gnuastro-0.2.33-8a3b/0000755000175000017500000000000013004464727011204 500000000000000gnuastro-0.2.33-8a3b/.tarball-version0000644000175000017500000000001413004464727014224 000000000000000.2.33-8a3b gnuastro-0.2.33-8a3b/tests/0000755000175000017500000000000013004464727012346 500000000000000gnuastro-0.2.33-8a3b/tests/during-dev.sh0000755000175000017500000001340113004133612014652 00000000000000#! /bin/sh # Script to rebuild and test a utility during development. # # During the development of Gnuastro, you often make changes in a utility # then need to rebuild and run it with special arguments and options (to # test your work). This script is made to facilitate this process. It will # take these steps: # # 1. Delete an existing utility executable. # # 2. Run Make on all Gnuastro. # # 3. If Make was successful, then go into the output directory, and run # utility with the given arguments and options. The executable is run # within an output directory (possibly different from the source or # build directories) so if you need to make lots of temporary test # files, there they won't get mixed up with non-output files. # # Combined with the `tmpfs-config-make', this script can be used to greatly # simplify the development process. After running that script once, for # subsequent builds during your development, you can run this script from # the top source directory (by running `./tests/during-dev.sh', or giving # this to the `compile' command in Emacs). Note that you have to set the # first few variables (directories, utility name, arguments and options) # manually before each major development activity. # # This file will be changed alot during development. So please make sure # you have left the variable values empty before committing. This will # remind each developer running this script to set the values based on # their particular work. Alternatively you can reset this file to its # version controlled status before committing your main work with the # command below: # # git checkout -- tests/during-dev.sh # # This file can also be used as a model to write a test for the work you # have done (to be checked with `make check'). Just copy and paste an # existing test from the utility and replace the last few lines based on # this file. # # Original author: # Mohammad Akhlaghi # Contributing author(s): # Copyright (C) 2016, Free Software Foundation, Inc. # # Gnuastro is free software: you can redistribute it and/or modify it under # the terms of the GNU General Public License as published by the Free # Software Foundation, either version 3 of the License, or (at your option) # any later version. # # Gnuastro is distributed in the hope that it will be useful, but WITHOUT # ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or # FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for # more details. # # You should have received a copy of the GNU General Public License along # with Gnuastro. If not, see . # SET INPUT PARAMETERS # ==================== # Set the basic test directories. If you are building over the source # directory, then set `builddir' to `./'. If you want the outputs to be in # the top source directory, set it to `./'. Since 'build' is the assumed # symbolic link in `tmpfs-config-make', it is also assumed in the version # controlled version of this script. Note, if your directory names have # space characters in them, quote the full value builddir=build outdir= # Set the utility name, along with its arguments and options. NOTE, for # multiple arguments and options, please put them all between quotation # marks so the space characters are included. If there are spaces in the # values of the options or arguments, quote them two times (once for this # script, and once for the utility. In such cases it might be easier to # just add the argument/option to the final script that runs the utility # rather than these variables. utilname= arguments= options= # RUN THE PROCEDURES # ================== # First, make sure the variables are set. Note that arguments and options # are not absolutly vital! so they are not checked here. The utility will # warn and halt if it needs them. if [ x"$outdir" = x ]; then echo "outdir is not set."; exit 1; fi if [ x$utilname = x ]; then echo "utilname is not set."; exit 1; fi if [ x"$builddir" = x ]; then echo "builddir is not set."; exit 1; fi # If builddir is relative, then append the current directory to make it # absolute. This is done because we will be going into the output directory # for executing the utility and we need to know the absolute address of the # top build directory. srcdir=$(pwd) if [ ! "${builddir:0:1}" = "/" ]; then builddir="$srcdir/$builddir" fi # Set the utility's executable file name utility="$builddir/bin/$utilname/ast$utilname" # If the utility is already built, then remove the executable so it is # definitely remade. if [ -f "$utility" ]; then rm "$utility"; fi # Make Gnuastro (note that during development, it is sometimes necessary to # edit/rebuild the libraries too). If Make is successful, then change to # the output directory and run the utility with the given arguments and # options. # # Before actually running put a copy of the configuration file in the # output directory and also add the onlydirconf option so user or system # wide configuration files don't interfere. if make -C "$builddir"; then # Change to the output directory. cd "$outdir" # Make the .gnuastro directory if it doesn't exist. if [ ! -d .gnuastro ]; then mkdir .gnuastro fi # Put a copy of this utility's configuration file there and add the # onlydirconf option. We are first printing an empty line just in case # the last line in the configuration file doesn't actualy end with a # new line (in which case the appended string will be added to the end # of the last line). cp "$srcdir/bin/$utilname/ast$utilname.conf" .gnuastro/ echo "" >> .gnuastro/ast$utilname.conf echo " onlydirconf 1" >> .gnuastro/ast$utilname.conf # Run the built utility with the given arguments and options. "$utility" $arguments $options fi gnuastro-0.2.33-8a3b/tests/prepconf.sh0000755000175000017500000000620212771240371014436 00000000000000# This is not actually a test of any of the programs, it just brings # in all the configuration files into a locally created .gnuastro # directory for all the tests to use. It is part of the GNU Astronomy # Utilities (Gnuastro). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # Copyright (C) 2016, Free Software Foundation, Inc. # # Gnuastro is free software: you can redistribute it and/or modify it # under the terms of the GNU General Public License as published by the # Free Software Foundation, either version 3 of the License, or (at your # option) any later version. # # Gnuastro is distributed in the hope that it will be useful, but # WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU # General Public License for more details. # # You should have received a copy of the GNU General Public License # along with Gnuastro. If not, see . # Make the .gnuastro directory # ---------------------------- # # This directory will keep all the utility configuration files for # this run of `make check'. if [ ! -d .gnuastro ]; then mkdir .gnuastro fi # Add options for `make check' # ---------------------------- # # It might be necessary to add specific options to all the programs during # `make check'. Therefore we have defined the file `addedoptions.txt' to # keep these extra options and append them to the configuration file in the # source directory of the utility. # # - The onlydirconf option is added so the utilities don't go looking # into the user's home and system wide directories (which might contain # configuration files from older versions). If the option names have # changed or an option has been removed, such sitations will cause a # failed test. # # - When checking on multiple threads, the log files generated by the # utilities can get mixed and cause failures, so it is better for the # utility test scripts to not generate any log files. In the utility # design, it is best that a fatal error is reported on the standard # error (which will be recorded in the test outputs), not in a log # file. However, a solution that would allow us to keep the log files # would be to make the log file names depend on the input filenames. cat > addedoptions.txt < .gnuastro/ast$prog.conf done # Clean up # -------- # # Delete the `addedoptions.txt' file that was generated here. rm addedoptions.txt gnuastro-0.2.33-8a3b/tests/multithread0000755000175000017500000001736013004464725014543 00000000000000#! /bin/sh # multithread - temporary wrapper script for .libs/multithread # Generated by libtool (GNU libtool) 2.4.6 # # The multithread program cannot be directly executed until all the libtool # libraries that it depends on are installed. # # This wrapper script should never be moved out of the build directory. # If it is, it will not operate correctly. # Sed substitution that helps us do robust quoting. It backslashifies # metacharacters that are still active within double-quoted strings. sed_quote_subst='s|\([`"$\\]\)|\\\1|g' # Be Bourne compatible if test -n "${ZSH_VERSION+set}" && (emulate sh) >/dev/null 2>&1; then emulate sh NULLCMD=: # Zsh 3.x and 4.x performs word splitting on ${1+"$@"}, which # is contrary to our usage. Disable this feature. alias -g '${1+"$@"}'='"$@"' setopt NO_GLOB_SUBST else case `(set -o) 2>/dev/null` in *posix*) set -o posix;; esac fi BIN_SH=xpg4; export BIN_SH # for Tru64 DUALCASE=1; export DUALCASE # for MKS sh # The HP-UX ksh and POSIX shell print the target directory to stdout # if CDPATH is set. (unset CDPATH) >/dev/null 2>&1 && unset CDPATH relink_command="(cd /home/mohammad/documents/personal/research/software/local/c/gnuastro/build/tests; { test -z \"\${LIBRARY_PATH+set}\" || unset LIBRARY_PATH || { LIBRARY_PATH=; export LIBRARY_PATH; }; }; { test -z \"\${COMPILER_PATH+set}\" || unset COMPILER_PATH || { COMPILER_PATH=; export COMPILER_PATH; }; }; { test -z \"\${GCC_EXEC_PREFIX+set}\" || unset GCC_EXEC_PREFIX || { GCC_EXEC_PREFIX=; export GCC_EXEC_PREFIX; }; }; { test -z \"\${LD_RUN_PATH+set}\" || unset LD_RUN_PATH || { LD_RUN_PATH=; export LD_RUN_PATH; }; }; LD_LIBRARY_PATH=:/usr/local/lib; export LD_LIBRARY_PATH; PATH=/usr/local/sbin:/usr/local/bin:/usr/bin:/usr/bin/site_perl:/usr/bin/vendor_perl:/usr/bin/core_perl:/usr/local/texlive/2016/bin/x86_64-linux; export PATH; gcc -Wall -O3 -pthread -pthread -o \$progdir/\$file lib/multithread.o -L../lib /home/mohammad/documents/personal/research/software/local/c/gnuastro/build/lib/.libs/libgnuastro.so -lgit2 -ljpeg -lwcs -lcfitsio /usr/local/lib/libgsl.so /usr/local/lib/libgslcblas.so -lm -pthread -Wl,-rpath -Wl,/home/mohammad/documents/personal/research/software/local/c/gnuastro/build/lib/.libs -Wl,-rpath -Wl,/usr/local/lib -Wl,-rpath -Wl,/usr/local/lib)" # This environment variable determines our operation mode. if test "$libtool_install_magic" = "%%%MAGIC variable%%%"; then # install mode needs the following variables: generated_by_libtool_version='2.4.6' notinst_deplibs=' /home/mohammad/documents/personal/research/software/local/c/gnuastro/build/lib/libgnuastro.la' else # When we are sourced in execute mode, $file and $ECHO are already set. if test "$libtool_execute_magic" != "%%%MAGIC variable%%%"; then file="$0" # A function that is used when there is no print builtin or printf. func_fallback_echo () { eval 'cat <<_LTECHO_EOF $1 _LTECHO_EOF' } ECHO="printf %s\\n" fi # Very basic option parsing. These options are (a) specific to # the libtool wrapper, (b) are identical between the wrapper # /script/ and the wrapper /executable/ that is used only on # windows platforms, and (c) all begin with the string --lt- # (application programs are unlikely to have options that match # this pattern). # # There are only two supported options: --lt-debug and # --lt-dump-script. There is, deliberately, no --lt-help. # # The first argument to this parsing function should be the # script's ../libtool value, followed by no. lt_option_debug= func_parse_lt_options () { lt_script_arg0=$0 shift for lt_opt do case "$lt_opt" in --lt-debug) lt_option_debug=1 ;; --lt-dump-script) lt_dump_D=`$ECHO "X$lt_script_arg0" | /usr/bin/sed -e 's/^X//' -e 's%/[^/]*$%%'` test "X$lt_dump_D" = "X$lt_script_arg0" && lt_dump_D=. lt_dump_F=`$ECHO "X$lt_script_arg0" | /usr/bin/sed -e 's/^X//' -e 's%^.*/%%'` cat "$lt_dump_D/$lt_dump_F" exit 0 ;; --lt-*) $ECHO "Unrecognized --lt- option: '$lt_opt'" 1>&2 exit 1 ;; esac done # Print the debug banner immediately: if test -n "$lt_option_debug"; then echo "multithread:multithread:$LINENO: libtool wrapper (GNU libtool) 2.4.6" 1>&2 fi } # Used when --lt-debug. Prints its arguments to stdout # (redirection is the responsibility of the caller) func_lt_dump_args () { lt_dump_args_N=1; for lt_arg do $ECHO "multithread:multithread:$LINENO: newargv[$lt_dump_args_N]: $lt_arg" lt_dump_args_N=`expr $lt_dump_args_N + 1` done } # Core function for launching the target application func_exec_program_core () { if test -n "$lt_option_debug"; then $ECHO "multithread:multithread:$LINENO: newargv[0]: $progdir/$program" 1>&2 func_lt_dump_args ${1+"$@"} 1>&2 fi exec "$progdir/$program" ${1+"$@"} $ECHO "$0: cannot exec $program $*" 1>&2 exit 1 } # A function to encapsulate launching the target application # Strips options in the --lt-* namespace from $@ and # launches target application with the remaining arguments. func_exec_program () { case " $* " in *\ --lt-*) for lt_wr_arg do case $lt_wr_arg in --lt-*) ;; *) set x "$@" "$lt_wr_arg"; shift;; esac shift done ;; esac func_exec_program_core ${1+"$@"} } # Parse options func_parse_lt_options "$0" ${1+"$@"} # Find the directory that this script lives in. thisdir=`$ECHO "$file" | /usr/bin/sed 's%/[^/]*$%%'` test "x$thisdir" = "x$file" && thisdir=. # Follow symbolic links until we get to the real thisdir. file=`ls -ld "$file" | /usr/bin/sed -n 's/.*-> //p'` while test -n "$file"; do destdir=`$ECHO "$file" | /usr/bin/sed 's%/[^/]*$%%'` # If there was a directory component, then change thisdir. if test "x$destdir" != "x$file"; then case "$destdir" in [\\/]* | [A-Za-z]:[\\/]*) thisdir="$destdir" ;; *) thisdir="$thisdir/$destdir" ;; esac fi file=`$ECHO "$file" | /usr/bin/sed 's%^.*/%%'` file=`ls -ld "$thisdir/$file" | /usr/bin/sed -n 's/.*-> //p'` done # Usually 'no', except on cygwin/mingw when embedded into # the cwrapper. WRAPPER_SCRIPT_BELONGS_IN_OBJDIR=no if test "$WRAPPER_SCRIPT_BELONGS_IN_OBJDIR" = "yes"; then # special case for '.' if test "$thisdir" = "."; then thisdir=`pwd` fi # remove .libs from thisdir case "$thisdir" in *[\\/].libs ) thisdir=`$ECHO "$thisdir" | /usr/bin/sed 's%[\\/][^\\/]*$%%'` ;; .libs ) thisdir=. ;; esac fi # Try to get the absolute directory name. absdir=`cd "$thisdir" && pwd` test -n "$absdir" && thisdir="$absdir" program=lt-'multithread' progdir="$thisdir/.libs" if test ! -f "$progdir/$program" || { file=`ls -1dt "$progdir/$program" "$progdir/../$program" 2>/dev/null | /usr/bin/sed 1q`; \ test "X$file" != "X$progdir/$program"; }; then file="$$-$program" if test ! -d "$progdir"; then mkdir "$progdir" else rm -f "$progdir/$file" fi # relink executable if necessary if test -n "$relink_command"; then if relink_command_output=`eval $relink_command 2>&1`; then : else $ECHO "$relink_command_output" >&2 rm -f "$progdir/$file" exit 1 fi fi mv -f "$progdir/$file" "$progdir/$program" 2>/dev/null || { rm -f "$progdir/$program"; mv -f "$progdir/$file" "$progdir/$program"; } rm -f "$progdir/$file" fi if test -f "$progdir/$program"; then if test "$libtool_execute_magic" != "%%%MAGIC variable%%%"; then # Run the actual program with our arguments. func_exec_program ${1+"$@"} fi else # The program doesn't exist. $ECHO "$0: error: '$progdir/$program' does not exist" 1>&2 $ECHO "This script is just a wrapper for $program." 1>&2 $ECHO "See the libtool documentation for more information." 1>&2 exit 1 fi fi gnuastro-0.2.33-8a3b/tests/arraymanip0000755000175000017500000001734513004464725014367 00000000000000#! /bin/sh # arraymanip - temporary wrapper script for .libs/arraymanip # Generated by libtool (GNU libtool) 2.4.6 # # The arraymanip program cannot be directly executed until all the libtool # libraries that it depends on are installed. # # This wrapper script should never be moved out of the build directory. # If it is, it will not operate correctly. # Sed substitution that helps us do robust quoting. It backslashifies # metacharacters that are still active within double-quoted strings. sed_quote_subst='s|\([`"$\\]\)|\\\1|g' # Be Bourne compatible if test -n "${ZSH_VERSION+set}" && (emulate sh) >/dev/null 2>&1; then emulate sh NULLCMD=: # Zsh 3.x and 4.x performs word splitting on ${1+"$@"}, which # is contrary to our usage. Disable this feature. alias -g '${1+"$@"}'='"$@"' setopt NO_GLOB_SUBST else case `(set -o) 2>/dev/null` in *posix*) set -o posix;; esac fi BIN_SH=xpg4; export BIN_SH # for Tru64 DUALCASE=1; export DUALCASE # for MKS sh # The HP-UX ksh and POSIX shell print the target directory to stdout # if CDPATH is set. (unset CDPATH) >/dev/null 2>&1 && unset CDPATH relink_command="(cd /home/mohammad/documents/personal/research/software/local/c/gnuastro/build/tests; { test -z \"\${LIBRARY_PATH+set}\" || unset LIBRARY_PATH || { LIBRARY_PATH=; export LIBRARY_PATH; }; }; { test -z \"\${COMPILER_PATH+set}\" || unset COMPILER_PATH || { COMPILER_PATH=; export COMPILER_PATH; }; }; { test -z \"\${GCC_EXEC_PREFIX+set}\" || unset GCC_EXEC_PREFIX || { GCC_EXEC_PREFIX=; export GCC_EXEC_PREFIX; }; }; { test -z \"\${LD_RUN_PATH+set}\" || unset LD_RUN_PATH || { LD_RUN_PATH=; export LD_RUN_PATH; }; }; LD_LIBRARY_PATH=:/usr/local/lib; export LD_LIBRARY_PATH; PATH=/usr/local/sbin:/usr/local/bin:/usr/bin:/usr/bin/site_perl:/usr/bin/vendor_perl:/usr/bin/core_perl:/usr/local/texlive/2016/bin/x86_64-linux; export PATH; gcc -Wall -O3 -pthread -pthread -o \$progdir/\$file lib/arraymanip.o -L../lib /home/mohammad/documents/personal/research/software/local/c/gnuastro/build/lib/.libs/libgnuastro.so -lgit2 -ljpeg -lwcs -lcfitsio /usr/local/lib/libgsl.so /usr/local/lib/libgslcblas.so -lm -pthread -Wl,-rpath -Wl,/home/mohammad/documents/personal/research/software/local/c/gnuastro/build/lib/.libs -Wl,-rpath -Wl,/usr/local/lib -Wl,-rpath -Wl,/usr/local/lib)" # This environment variable determines our operation mode. if test "$libtool_install_magic" = "%%%MAGIC variable%%%"; then # install mode needs the following variables: generated_by_libtool_version='2.4.6' notinst_deplibs=' /home/mohammad/documents/personal/research/software/local/c/gnuastro/build/lib/libgnuastro.la' else # When we are sourced in execute mode, $file and $ECHO are already set. if test "$libtool_execute_magic" != "%%%MAGIC variable%%%"; then file="$0" # A function that is used when there is no print builtin or printf. func_fallback_echo () { eval 'cat <<_LTECHO_EOF $1 _LTECHO_EOF' } ECHO="printf %s\\n" fi # Very basic option parsing. These options are (a) specific to # the libtool wrapper, (b) are identical between the wrapper # /script/ and the wrapper /executable/ that is used only on # windows platforms, and (c) all begin with the string --lt- # (application programs are unlikely to have options that match # this pattern). # # There are only two supported options: --lt-debug and # --lt-dump-script. There is, deliberately, no --lt-help. # # The first argument to this parsing function should be the # script's ../libtool value, followed by no. lt_option_debug= func_parse_lt_options () { lt_script_arg0=$0 shift for lt_opt do case "$lt_opt" in --lt-debug) lt_option_debug=1 ;; --lt-dump-script) lt_dump_D=`$ECHO "X$lt_script_arg0" | /usr/bin/sed -e 's/^X//' -e 's%/[^/]*$%%'` test "X$lt_dump_D" = "X$lt_script_arg0" && lt_dump_D=. lt_dump_F=`$ECHO "X$lt_script_arg0" | /usr/bin/sed -e 's/^X//' -e 's%^.*/%%'` cat "$lt_dump_D/$lt_dump_F" exit 0 ;; --lt-*) $ECHO "Unrecognized --lt- option: '$lt_opt'" 1>&2 exit 1 ;; esac done # Print the debug banner immediately: if test -n "$lt_option_debug"; then echo "arraymanip:arraymanip:$LINENO: libtool wrapper (GNU libtool) 2.4.6" 1>&2 fi } # Used when --lt-debug. Prints its arguments to stdout # (redirection is the responsibility of the caller) func_lt_dump_args () { lt_dump_args_N=1; for lt_arg do $ECHO "arraymanip:arraymanip:$LINENO: newargv[$lt_dump_args_N]: $lt_arg" lt_dump_args_N=`expr $lt_dump_args_N + 1` done } # Core function for launching the target application func_exec_program_core () { if test -n "$lt_option_debug"; then $ECHO "arraymanip:arraymanip:$LINENO: newargv[0]: $progdir/$program" 1>&2 func_lt_dump_args ${1+"$@"} 1>&2 fi exec "$progdir/$program" ${1+"$@"} $ECHO "$0: cannot exec $program $*" 1>&2 exit 1 } # A function to encapsulate launching the target application # Strips options in the --lt-* namespace from $@ and # launches target application with the remaining arguments. func_exec_program () { case " $* " in *\ --lt-*) for lt_wr_arg do case $lt_wr_arg in --lt-*) ;; *) set x "$@" "$lt_wr_arg"; shift;; esac shift done ;; esac func_exec_program_core ${1+"$@"} } # Parse options func_parse_lt_options "$0" ${1+"$@"} # Find the directory that this script lives in. thisdir=`$ECHO "$file" | /usr/bin/sed 's%/[^/]*$%%'` test "x$thisdir" = "x$file" && thisdir=. # Follow symbolic links until we get to the real thisdir. file=`ls -ld "$file" | /usr/bin/sed -n 's/.*-> //p'` while test -n "$file"; do destdir=`$ECHO "$file" | /usr/bin/sed 's%/[^/]*$%%'` # If there was a directory component, then change thisdir. if test "x$destdir" != "x$file"; then case "$destdir" in [\\/]* | [A-Za-z]:[\\/]*) thisdir="$destdir" ;; *) thisdir="$thisdir/$destdir" ;; esac fi file=`$ECHO "$file" | /usr/bin/sed 's%^.*/%%'` file=`ls -ld "$thisdir/$file" | /usr/bin/sed -n 's/.*-> //p'` done # Usually 'no', except on cygwin/mingw when embedded into # the cwrapper. 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GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ REPLACE_READ = @REPLACE_READ@ REPLACE_READLINK = @REPLACE_READLINK@ REPLACE_READLINKAT = @REPLACE_READLINKAT@ REPLACE_REALLOC = @REPLACE_REALLOC@ REPLACE_REALPATH = @REPLACE_REALPATH@ REPLACE_REMAINDER = @REPLACE_REMAINDER@ REPLACE_REMAINDERF = @REPLACE_REMAINDERF@ REPLACE_REMAINDERL = @REPLACE_REMAINDERL@ REPLACE_REMOVE = @REPLACE_REMOVE@ REPLACE_RENAME = @REPLACE_RENAME@ REPLACE_RENAMEAT = @REPLACE_RENAMEAT@ REPLACE_RMDIR = @REPLACE_RMDIR@ REPLACE_ROUND = @REPLACE_ROUND@ REPLACE_ROUNDF = @REPLACE_ROUNDF@ REPLACE_ROUNDL = @REPLACE_ROUNDL@ REPLACE_SETENV = @REPLACE_SETENV@ REPLACE_SETLOCALE = @REPLACE_SETLOCALE@ REPLACE_SIGNBIT = @REPLACE_SIGNBIT@ REPLACE_SIGNBIT_USING_GCC = @REPLACE_SIGNBIT_USING_GCC@ REPLACE_SLEEP = @REPLACE_SLEEP@ REPLACE_SNPRINTF = @REPLACE_SNPRINTF@ REPLACE_SPRINTF = @REPLACE_SPRINTF@ REPLACE_SQRTL = @REPLACE_SQRTL@ REPLACE_STAT = @REPLACE_STAT@ REPLACE_STDIO_READ_FUNCS = @REPLACE_STDIO_READ_FUNCS@ REPLACE_STDIO_WRITE_FUNCS = @REPLACE_STDIO_WRITE_FUNCS@ REPLACE_STPNCPY = @REPLACE_STPNCPY@ REPLACE_STRCASESTR = @REPLACE_STRCASESTR@ REPLACE_STRCHRNUL = @REPLACE_STRCHRNUL@ REPLACE_STRDUP = @REPLACE_STRDUP@ REPLACE_STRERROR = @REPLACE_STRERROR@ REPLACE_STRERROR_R = @REPLACE_STRERROR_R@ REPLACE_STRNCAT = @REPLACE_STRNCAT@ REPLACE_STRNDUP = @REPLACE_STRNDUP@ REPLACE_STRNLEN = @REPLACE_STRNLEN@ REPLACE_STRSIGNAL = @REPLACE_STRSIGNAL@ REPLACE_STRSTR = @REPLACE_STRSTR@ REPLACE_STRTOD = @REPLACE_STRTOD@ REPLACE_STRTOIMAX = @REPLACE_STRTOIMAX@ REPLACE_STRTOK_R = @REPLACE_STRTOK_R@ REPLACE_STRTOUMAX = @REPLACE_STRTOUMAX@ REPLACE_STRUCT_LCONV = @REPLACE_STRUCT_LCONV@ REPLACE_STRUCT_TIMEVAL = @REPLACE_STRUCT_TIMEVAL@ REPLACE_SYMLINK = @REPLACE_SYMLINK@ REPLACE_SYMLINKAT = @REPLACE_SYMLINKAT@ REPLACE_TIMEGM = @REPLACE_TIMEGM@ REPLACE_TMPFILE = @REPLACE_TMPFILE@ REPLACE_TOWLOWER = @REPLACE_TOWLOWER@ REPLACE_TRUNC = @REPLACE_TRUNC@ REPLACE_TRUNCF = @REPLACE_TRUNCF@ REPLACE_TRUNCL = @REPLACE_TRUNCL@ REPLACE_TTYNAME_R = @REPLACE_TTYNAME_R@ REPLACE_UNLINK = @REPLACE_UNLINK@ REPLACE_UNLINKAT = @REPLACE_UNLINKAT@ REPLACE_UNSETENV = @REPLACE_UNSETENV@ REPLACE_USLEEP = @REPLACE_USLEEP@ REPLACE_UTIMENSAT = @REPLACE_UTIMENSAT@ REPLACE_VASPRINTF = @REPLACE_VASPRINTF@ REPLACE_VDPRINTF = @REPLACE_VDPRINTF@ REPLACE_VFPRINTF = @REPLACE_VFPRINTF@ REPLACE_VPRINTF = @REPLACE_VPRINTF@ REPLACE_VSNPRINTF = @REPLACE_VSNPRINTF@ REPLACE_VSPRINTF = @REPLACE_VSPRINTF@ REPLACE_WCRTOMB = @REPLACE_WCRTOMB@ REPLACE_WCSNRTOMBS = @REPLACE_WCSNRTOMBS@ REPLACE_WCSRTOMBS = @REPLACE_WCSRTOMBS@ REPLACE_WCSWIDTH = @REPLACE_WCSWIDTH@ REPLACE_WCTOB = @REPLACE_WCTOB@ REPLACE_WCTOMB = @REPLACE_WCTOMB@ REPLACE_WCWIDTH = @REPLACE_WCWIDTH@ REPLACE_WRITE = @REPLACE_WRITE@ SED = @SED@ SET_MAKE = @SET_MAKE@ SHELL = @SHELL@ SIG_ATOMIC_T_SUFFIX = @SIG_ATOMIC_T_SUFFIX@ SIZE_T_SUFFIX = @SIZE_T_SUFFIX@ STDALIGN_H = @STDALIGN_H@ STDBOOL_H = @STDBOOL_H@ STDDEF_H = @STDDEF_H@ STDINT_H = @STDINT_H@ STRIP = @STRIP@ SYSEXITS_H = @SYSEXITS_H@ SYS_TIME_H_DEFINES_STRUCT_TIMESPEC = @SYS_TIME_H_DEFINES_STRUCT_TIMESPEC@ TIME_H_DEFINES_STRUCT_TIMESPEC = @TIME_H_DEFINES_STRUCT_TIMESPEC@ UINT32_MAX_LT_UINTMAX_MAX = @UINT32_MAX_LT_UINTMAX_MAX@ UINT64_MAX_EQ_ULONG_MAX = @UINT64_MAX_EQ_ULONG_MAX@ UNDEFINE_STRTOK_R = @UNDEFINE_STRTOK_R@ UNISTD_H_DEFINES_STRUCT_TIMESPEC = @UNISTD_H_DEFINES_STRUCT_TIMESPEC@ UNISTD_H_HAVE_WINSOCK2_H = @UNISTD_H_HAVE_WINSOCK2_H@ UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS = @UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS@ VERSION = @VERSION@ WCHAR_T_SUFFIX = @WCHAR_T_SUFFIX@ WINDOWS_64_BIT_OFF_T = @WINDOWS_64_BIT_OFF_T@ WINDOWS_64_BIT_ST_SIZE = @WINDOWS_64_BIT_ST_SIZE@ WINT_T_SUFFIX = @WINT_T_SUFFIX@ YIELD_LIB = @YIELD_LIB@ abs_builddir = @abs_builddir@ abs_srcdir = @abs_srcdir@ abs_top_builddir = @abs_top_builddir@ abs_top_srcdir = @abs_top_srcdir@ ac_ct_AR = @ac_ct_AR@ ac_ct_CC = @ac_ct_CC@ ac_ct_CXX = @ac_ct_CXX@ ac_ct_DUMPBIN = @ac_ct_DUMPBIN@ am__include = @am__include@ am__leading_dot = @am__leading_dot@ am__quote = @am__quote@ am__tar = @am__tar@ am__untar = @am__untar@ ax_pthread_config = @ax_pthread_config@ bindir = @bindir@ build = @build@ build_alias = @build_alias@ build_cpu = @build_cpu@ build_os = @build_os@ build_vendor = @build_vendor@ builddir = @builddir@ datadir = @datadir@ datarootdir = @datarootdir@ docdir = @docdir@ dvidir = @dvidir@ exec_prefix = @exec_prefix@ gl_LIBOBJS = @gl_LIBOBJS@ gl_LTLIBOBJS = @gl_LTLIBOBJS@ gltests_LIBOBJS = @gltests_LIBOBJS@ gltests_LTLIBOBJS = @gltests_LTLIBOBJS@ gltests_WITNESS = @gltests_WITNESS@ has_ghostscript = @has_ghostscript@ has_help2man = @has_help2man@ host = @host@ host_alias = @host_alias@ host_cpu = @host_cpu@ host_os = @host_os@ host_vendor = @host_vendor@ htmldir = @htmldir@ includedir = @includedir@ infodir = @infodir@ install_sh = @install_sh@ libdir = @libdir@ libexecdir = @libexecdir@ lispdir = @lispdir@ localedir = @localedir@ localstatedir = @localstatedir@ mandir = @mandir@ mkdir_p = @mkdir_p@ oldincludedir = @oldincludedir@ pdfdir = @pdfdir@ prefix = @prefix@ program_transform_name = @program_transform_name@ psdir = @psdir@ runstatedir = @runstatedir@ sbindir = @sbindir@ sharedstatedir = @sharedstatedir@ srcdir = @srcdir@ sysconfdir = @sysconfdir@ target_alias = @target_alias@ top_build_prefix = @top_build_prefix@ top_builddir = @top_builddir@ top_srcdir = @top_srcdir@ # Translate conditions that came from `./configure' into variables that can # be used here. @COND_HASGHOSTSCRIPT_TRUE@MAYBE_HASGHOSTSCRIPT = "yes" @COND_HASLIBJPEG_TRUE@MAYBE_HASLIBJPEG = "yes" # `gnuastro.h' is built by `../lib/Makefile.am' and is only meant for # outside users (internally `config.h' has everything. Thus, we need to add # it to the include directories of the test programs in this directory. AM_CPPFLAGS = -I../lib # Environment variables for the test scripts. AM_TESTS_ENVIRONMENT = \ export topsrc=$(top_srcdir); \ export haslibjpeg=$(MAYBE_HASLIBJPEG); \ export hasghostscript=$(MAYBE_HASGHOSTSCRIPT); # Compilations that are to be done with `make check'. 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See "Extending Automake # rules", and the "What Gets Cleaned" sections of the Automake manual. clean-local:; rm -rf .gnuastro mkprof/mosaic1.sh: prepconf.sh.log mkprof/mosaic2.sh: prepconf.sh.log mkprof/mosaic3.sh: prepconf.sh.log mkprof/mosaic4.sh: prepconf.sh.log mkprof/radeccat.sh: prepconf.sh.log table/asciitobinary.sh: prepconf.sh.log table/binarytoascii.sh: table/asciitobinary.sh.log imgcrop/imgcat.sh: mkprof/mosaic1.sh.log imgcrop/wcscat.sh: mkprof/mosaic1.sh.log mkprof/mosaic2.sh.log \ mkprof/mosaic3.sh.log mkprof/mosaic4.sh.log imgcrop/xcyc.sh: mkprof/mosaic1.sh.log imgcrop/xcycnoblank.sh: mkprof/mosaic1.sh.log imgcrop/section.sh: mkprof/mosaic1.sh.log imgcrop/radec.sh: mkprof/mosaic1.sh.log mkprof/mosaic2.sh.log \ mkprof/mosaic3.sh.log mkprof/mosaic4.sh.log imgcrop/imgpolygon.sh: mkprof/mosaic1.sh.log imgcrop/imgoutpolygon.sh: mkprof/mosaic1.sh.log imgcrop/wcspolygon.sh: mkprof/mosaic1.sh.log mkprof/mosaic2.sh.log \ mkprof/mosaic3.sh.log mkprof/mosaic4.sh.log convertt/fitstotxt.sh: mkprof/mosaic1.sh.log convertt/fitstojpeg.sh: mkprof/mosaic1.sh.log convertt/blankch.sh: mkprof/mosaic1.sh.log convertt/jpegtotxt.sh: convertt/fitstojpeg.sh.log convertt/fitstojpegcmyk.sh: mkprof/mosaic1.sh.log convertt/jpegtofits.sh: convertt/blankch.sh.log convertt/fitstopdf.sh: imgcrop/section.sh.log convolve/spatial.sh: mkprof/mosaic1.sh.log convolve/frequency.sh: mkprof/mosaic1.sh.log imgwarp/imgwarp_scale.sh: convolve/spatial.sh.log imgwarp/homographic.sh: convolve/spatial.sh.log mknoise/addnoise.sh: imgwarp/imgwarp_scale.sh.log mkprof/ellipticalmasks.sh: mknoise/addnoise.sh.log mkprof/inputascanvas.sh: mknoise/addnoise.sh.log header/write.sh: convolve/spatial.sh.log header/print.sh: header/write.sh.log header/update.sh: header/write.sh.log header/delete.sh: header/write.sh.log imgstat/basicstats.sh: mknoise/addnoise.sh.log subtractsky/subtractsky.sh: mknoise/addnoise.sh.log noisechisel/noisechisel.sh: mknoise/addnoise.sh.log mkcatalog/simple.sh: noisechisel/noisechisel.sh.log mkcatalog/aperturephot.sh: noisechisel/noisechisel.sh.log \ mkprof/inputascanvas.sh arithmetic/snimage.sh: noisechisel/noisechisel.sh.log arithmetic/where.sh: noisechisel/noisechisel.sh.log arithmetic/or.sh: noisechisel/noisechisel.sh.log arithmetic/onlynumbers.sh: prepconf.sh.log cosmiccal/simpletest.sh: prepconf.sh.log # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: gnuastro-0.2.33-8a3b/tests/Makefile.am0000644000175000017500000001505112770772473014335 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . # Translate conditions that came from `./configure' into variables that can # be used here. if COND_HASGHOSTSCRIPT MAYBE_HASGHOSTSCRIPT = "yes" endif if COND_HASLIBJPEG MAYBE_HASLIBJPEG = "yes" endif # `gnuastro.h' is built by `../lib/Makefile.am' and is only meant for # outside users (internally `config.h' has everything. Thus, we need to add # it to the include directories of the test programs in this directory. AM_CPPFLAGS = -I../lib # Environment variables for the test scripts. AM_TESTS_ENVIRONMENT = \ export topsrc=$(top_srcdir); \ export haslibjpeg=$(MAYBE_HASLIBJPEG); \ export hasghostscript=$(MAYBE_HASGHOSTSCRIPT); # Compilations that are to be done with `make check'. LDADD = -lgnuastro check_PROGRAMS = versioncpp arraymanip multithread arraymanip_SOURCES = lib/arraymanip.c versioncpp_SOURCES = lib/versioncpp.cpp multithread_SOURCES = lib/multithread.c # The actual test scripts that are run: TESTS = $(check_PROGRAMS) prepconf.sh mkprof/mosaic1.sh mkprof/mosaic2.sh \ mkprof/mosaic3.sh mkprof/mosaic4.sh mkprof/radeccat.sh imgcrop/imgcat.sh \ imgcrop/wcscat.sh imgcrop/xcyc.sh imgcrop/xcycnoblank.sh \ imgcrop/section.sh imgcrop/radec.sh imgcrop/imgpolygon.sh \ imgcrop/imgoutpolygon.sh imgcrop/wcspolygon.sh convertt/fitstotxt.sh \ convertt/fitstojpeg.sh convertt/blankch.sh convertt/jpegtotxt.sh \ convertt/fitstojpegcmyk.sh convertt/jpegtofits.sh convertt/fitstopdf.sh \ convolve/spatial.sh convolve/frequency.sh imgwarp/imgwarp_scale.sh \ imgwarp/homographic.sh mknoise/addnoise.sh mkprof/ellipticalmasks.sh \ mkprof/inputascanvas.sh header/write.sh header/print.sh header/update.sh \ header/delete.sh imgstat/basicstats.sh subtractsky/subtractsky.sh \ noisechisel/noisechisel.sh mkcatalog/simple.sh mkcatalog/aperturephot.sh \ arithmetic/snimage.sh arithmetic/onlynumbers.sh arithmetic/where.sh \ arithmetic/or.sh cosmiccal/simpletest.sh table/asciitobinary.sh \ table/binarytoascii.sh # Files to distribute along with the tests. EXTRA_DIST = $(TESTS) during-dev.sh mkprof/mkprofcat1.txt \ mkprof/ellipticalmasks.txt mkprof/inputascanvas.txt \ mkprof/mkprofcat2.txt mkprof/mkprofcat3.txt mkprof/mkprofcat4.txt \ mkprof/radeccat.txt imgcrop/cat.txt table/asciitobinary.txt # Files that must be cleaned with `make clean'. CLEANFILES = *.log *.txt *.jpg *.fits *.pdf *.eps # CLEANFILES is only for files, not directories. Therefore we are using # Automake's extending rules to clean the temporary `.gnuastro' directory # that was built by the `prepconf.sh' scripot. See "Extending Automake # rules", and the "What Gets Cleaned" sections of the Automake manual. clean-local:; rm -rf .gnuastro ## Dependency structure ## ==================== ## ## When run with `-jN' option, the tests can be run in parallel, so we need ## to define their dependencies on each other here. The output of all the ## tests that should be used (is recognized by Automake and will not mess ## the system) is the name of the test file appended by a `.log'. It ## contains the output of the program on standard output and error. THIS IS ## IMPORTANT: So even if the program fails, the .log file is created. The ## check if the input for a test exists or not should be checked in the ## test that depends on it, it can't be done here in the Makefile. mkprof/mosaic1.sh: prepconf.sh.log mkprof/mosaic2.sh: prepconf.sh.log mkprof/mosaic3.sh: prepconf.sh.log mkprof/mosaic4.sh: prepconf.sh.log mkprof/radeccat.sh: prepconf.sh.log table/asciitobinary.sh: prepconf.sh.log table/binarytoascii.sh: table/asciitobinary.sh.log imgcrop/imgcat.sh: mkprof/mosaic1.sh.log imgcrop/wcscat.sh: mkprof/mosaic1.sh.log mkprof/mosaic2.sh.log \ mkprof/mosaic3.sh.log mkprof/mosaic4.sh.log imgcrop/xcyc.sh: mkprof/mosaic1.sh.log imgcrop/xcycnoblank.sh: mkprof/mosaic1.sh.log imgcrop/section.sh: mkprof/mosaic1.sh.log imgcrop/radec.sh: mkprof/mosaic1.sh.log mkprof/mosaic2.sh.log \ mkprof/mosaic3.sh.log mkprof/mosaic4.sh.log imgcrop/imgpolygon.sh: mkprof/mosaic1.sh.log imgcrop/imgoutpolygon.sh: mkprof/mosaic1.sh.log imgcrop/wcspolygon.sh: mkprof/mosaic1.sh.log mkprof/mosaic2.sh.log \ mkprof/mosaic3.sh.log mkprof/mosaic4.sh.log convertt/fitstotxt.sh: mkprof/mosaic1.sh.log convertt/fitstojpeg.sh: mkprof/mosaic1.sh.log convertt/blankch.sh: mkprof/mosaic1.sh.log convertt/jpegtotxt.sh: convertt/fitstojpeg.sh.log convertt/fitstojpegcmyk.sh: mkprof/mosaic1.sh.log convertt/jpegtofits.sh: convertt/blankch.sh.log convertt/fitstopdf.sh: imgcrop/section.sh.log convolve/spatial.sh: mkprof/mosaic1.sh.log convolve/frequency.sh: mkprof/mosaic1.sh.log imgwarp/imgwarp_scale.sh: convolve/spatial.sh.log imgwarp/homographic.sh: convolve/spatial.sh.log mknoise/addnoise.sh: imgwarp/imgwarp_scale.sh.log mkprof/ellipticalmasks.sh: mknoise/addnoise.sh.log mkprof/inputascanvas.sh: mknoise/addnoise.sh.log header/write.sh: convolve/spatial.sh.log header/print.sh: header/write.sh.log header/update.sh: header/write.sh.log header/delete.sh: header/write.sh.log imgstat/basicstats.sh: mknoise/addnoise.sh.log subtractsky/subtractsky.sh: mknoise/addnoise.sh.log noisechisel/noisechisel.sh: mknoise/addnoise.sh.log mkcatalog/simple.sh: noisechisel/noisechisel.sh.log mkcatalog/aperturephot.sh: noisechisel/noisechisel.sh.log \ mkprof/inputascanvas.sh arithmetic/snimage.sh: noisechisel/noisechisel.sh.log arithmetic/where.sh: noisechisel/noisechisel.sh.log arithmetic/or.sh: noisechisel/noisechisel.sh.log arithmetic/onlynumbers.sh: prepconf.sh.log cosmiccal/simpletest.sh: prepconf.sh.log gnuastro-0.2.33-8a3b/tests/table/0000755000175000017500000000000013004464727013435 500000000000000gnuastro-0.2.33-8a3b/tests/table/asciitobinary.txt0000644000175000017500000000003312757417261016757 000000000000001 2.323 43.34 2 3213 1232 gnuastro-0.2.33-8a3b/tests/table/binarytoascii.sh0000755000175000017500000000230712771240370016552 00000000000000# Convert an ASCII table to a binary table # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=table execname=../bin/$prog/ast$prog table=asciitobinary.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $table --output=binarytoascii.txt -h1 gnuastro-0.2.33-8a3b/tests/table/asciitobinary.sh0000755000175000017500000000232713001143061016536 00000000000000# Convert an ASCII table to a binary table # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=table execname=../bin/$prog/ast$prog table=$topsrc/tests/$prog/asciitobinary.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $table --output=asciitobinary.fits gnuastro-0.2.33-8a3b/tests/subtractsky/0000755000175000017500000000000013004464727014724 500000000000000gnuastro-0.2.33-8a3b/tests/subtractsky/subtractsky.sh0000755000175000017500000000232712771240370017561 00000000000000# Add noise to a large image then subtract the sky. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=subtractsky execname=../bin/$prog/ast$prog img=convolve_spatial_noised.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $img --checksky --numnearest=4 gnuastro-0.2.33-8a3b/tests/noisechisel/0000755000175000017500000000000013004464727014653 500000000000000gnuastro-0.2.33-8a3b/tests/noisechisel/noisechisel.sh0000755000175000017500000000235112771240347017440 00000000000000# Detect objects and clumps in an image using NoiseChisel. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=noisechisel execname=../bin/$prog/ast$prog img=convolve_spatial_noised.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $img --checkdetection --checksegmentation gnuastro-0.2.33-8a3b/tests/mkprof/0000755000175000017500000000000013004464727013644 500000000000000gnuastro-0.2.33-8a3b/tests/mkprof/radeccat.txt0000644000175000017500000000076712752703246016106 00000000000000# Random catalog generated by makerandomcat.py # Column 0: ID # Column 1: X # Column 2: Y # Column 3: Function (0: Sersic, 1: Moffat, 2: Gaussian, 3: Point). # Column 4: Effective radius # Column 5: Sersic index. # Column 6: Position angle # Column 7: Axis ratio # Column 8: Magnitude # Column 9: Truncation radius 1 0.99987331 1.0001617 0 10.00 2.500 45.000 0.3 -6.0 2.000 2 0.99929656 1.0006917 0 10.00 2.500 135.00 0.3 -6.0 2.000 gnuastro-0.2.33-8a3b/tests/mkprof/mkprofcat4.txt0000644000175000017500000000013012536016724016370 000000000000001 0.40 0.40 0 20.00 2.500 45.000 1.00 -18.0 5.000 gnuastro-0.2.33-8a3b/tests/mkprof/mkprofcat3.txt0000644000175000017500000000013212536016716016372 000000000000001 100.40 0.40 0 20.00 2.500 45.000 1.00 -18.0 5.000 gnuastro-0.2.33-8a3b/tests/mkprof/mkprofcat2.txt0000644000175000017500000000013312536016706016371 000000000000001 0.400 100.40 0 20.00 2.500 45.000 1.00 -18.0 5.000 gnuastro-0.2.33-8a3b/tests/mkprof/inputascanvas.txt0000644000175000017500000000055412754576622017221 00000000000000# Column 0: ID # Column 1: X # Column 2: Y # Column 3: Function (0: Sersic, 1: Moffat, 2: Gaussian, 3: Point). # Column 4: Effective radius # Column 5: Sersic index. # Column 6: Position angle # Column 7: Axis ratio # Column 8: Magnitude # Column 9: Truncation radius 1 100.40 100.40 4 20.00 1 45.000 1.000 1 2.000 2 50.321 50.827 4 5.978 1 77.650 0.801 2 2.000 gnuastro-0.2.33-8a3b/tests/mkprof/ellipticalmasks.txt0000644000175000017500000000070112753412267017506 00000000000000# Column 0: ID # Column 1: X # Column 2: Y # Column 3: Function (0: Sersic, 1: Moffat, 2: Gaussian, 3: Point). # Column 4: Effective radius # Column 5: Sersic index. # Column 6: Position angle # Column 7: Axis ratio # Column 8: Magnitude # Column 9: Truncation radius 1 100.40 100.40 5 20.00 2.500 45.000 1.000 NaN 2.000 2 50.321 50.827 4 5.978 1.320 77.650 0.801 -1 2.000 gnuastro-0.2.33-8a3b/tests/mkprof/mkprofcat1.txt0000644000175000017500000000112212536016426016366 00000000000000# Random catalog generated by makerandomcat.py # Column 0: ID # Column 1: X # Column 2: Y # Column 3: Function (0: Sersic, 1: Moffat, 2: Gaussian, 3: Point). # Column 4: Effective radius # Column 5: Sersic index. # Column 6: Position angle # Column 7: Axis ratio # Column 8: Magnitude # Column 9: Truncation radius 1 0.0000 0.0000 1 3.000 4.765 0.0000 1.000 0.000 5.000 2 100.40 100.40 0 20.00 2.500 45.000 1.000 -18.0 5.000 3 50.321 50.827 0 5.978 1.320 77.650 0.801 -15.0 5.000 gnuastro-0.2.33-8a3b/tests/mkprof/inputascanvas.sh0000755000175000017500000000247612771240366017014 00000000000000# Make labeled regions on an image with blank pixels. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkprof execname=../bin/$prog/ast$prog img=convolve_spatial_noised.fits cat=$topsrc/tests/$prog/inputascanvas.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $cat $img --mforflatpix --inputascanvas \ --type=long --output="inputascanvas.fits" gnuastro-0.2.33-8a3b/tests/mkprof/ellipticalmasks.sh0000755000175000017500000000251212771240366017305 00000000000000# Make two masks (one flat and one circumference) cat1.txt # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkprof execname=../bin/$prog/ast$prog img=convolve_spatial_warped_noised.fits cat=$topsrc/tests/$prog/ellipticalmasks.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $cat $img --mforflatpix --replace --oversample=1 \ --output="ellipticalmasks.fits" gnuastro-0.2.33-8a3b/tests/mkprof/radeccat.sh0000755000175000017500000000215412771240366015674 00000000000000# Create a mock image from radeccat.txt # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkprof execname=../bin/$prog/ast$prog cat=$topsrc/tests/$prog/radeccat.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # if [ ! -f $execname ]; then exit 77; fi # Actual test script # ================== $execname $cat --racol=1 --deccol=2 --naxis1=100 --naxis2=100 gnuastro-0.2.33-8a3b/tests/mkprof/mosaic4.sh0000755000175000017500000000242612771240367015470 00000000000000# Create a mock image from cat2.txt: # # - It doesn't have any random profiles, only the large profile from # cat1.txt. The central position is set to be on the same real # place as in cat1.txt # # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkprof execname=../bin/$prog/ast$prog cat=$topsrc/tests/$prog/mkprofcat4.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # if [ ! -f $execname ]; then exit 77; fi # Actual test script # ================== $execname $cat --naxis1=100 --naxis2=100 --crpix1=-99 --crpix2=-99 gnuastro-0.2.33-8a3b/tests/mkprof/mosaic3.sh0000755000175000017500000000241112771240367015461 00000000000000# Create a mock image from cat2.txt: # # - It doesn't have any random profiles, only the large profile from # cat1.txt. The central position is set to be on the same real # place as in cat1.txt # # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkprof execname=../bin/$prog/ast$prog cat=$topsrc/tests/$prog/mkprofcat3.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # if [ ! -f $execname ]; then exit 77; fi # Actual test script # ================== $execname $cat --naxis1=100 --naxis2=100 --crpix2=-99 gnuastro-0.2.33-8a3b/tests/mkprof/mosaic2.sh0000755000175000017500000000250412771240367015463 00000000000000# Create a mock image from cat2.txt: # # - It doesn't have any random profiles, only the large profile from # cat1.txt. The central position is set to be on the same real # place as in cat1.txt # # - Also here, test the individual option. # # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkprof execname=../bin/$prog/ast$prog cat=$topsrc/tests/$prog/mkprofcat2.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # if [ ! -f $execname ]; then exit 77; fi # Actual test script # ================== $execname $cat --naxis1=100 --naxis2=100 --crpix1=-99 --individual gnuastro-0.2.33-8a3b/tests/mkprof/mosaic1.sh0000755000175000017500000000244612771240367015467 00000000000000# Create a mock image from cat1.txt: # # - It includes one large and bright profile that is on the last # pixel of this image. The other tests will also build the same # profile with the absolute place fixed. # # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkprof execname=../bin/$prog/ast$prog cat=$topsrc/tests/$prog/mkprofcat1.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # if [ ! -f $execname ]; then exit 77; fi # Actual test script # ================== $execname $cat --naxis1=100 --naxis2=100 mv 0_mkprofcat1.fits psf.fits gnuastro-0.2.33-8a3b/tests/mknoise/0000755000175000017500000000000013004464727014013 500000000000000gnuastro-0.2.33-8a3b/tests/mknoise/addnoise.sh0000755000175000017500000000315412771240364016062 00000000000000# Add noise to an input image. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). # # We will be adding noise to two images: the warped (smaller) and unwarped # (larger) mock images. The warped one will be used by programs that don't # care about the size of the image, but the larger one will be used by # those that do: for example SubtractSky and NoiseChisel will be better # tested on a larger image. prog=mknoise img1=convolve_spatial.fits execname=../bin/$prog/ast$prog img2=convolve_spatial_warped.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img1 ] || [ ! -f $img2 ]; then exit 77; fi # Actual test script # ================== export GSL_RNG_SEED=1 export GSL_RNG_TYPE=ranlxs2 $execname --envseed $img1 $execname --envseed $img2 gnuastro-0.2.33-8a3b/tests/mkcatalog/0000755000175000017500000000000013004464727014310 500000000000000gnuastro-0.2.33-8a3b/tests/mkcatalog/aperturephot.sh0000755000175000017500000000250312771240362017306 00000000000000# Make a simple catalog for NoiseChisel's output. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkcatalog objimg=inputascanvas.fits execname=../bin/$prog/ast$prog img=convolve_spatial_noised_labeled.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $img --objlabs=$objimg --objhdu=0 --output=aperturephot.txt \ --sn --magnitude --dec --ra --y --x gnuastro-0.2.33-8a3b/tests/mkcatalog/simple.sh0000755000175000017500000000236512774010036016057 00000000000000# Make a simple catalog for NoiseChisel's output. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkcatalog execname=../bin/$prog/ast$prog img=convolve_spatial_noised_labeled.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $img --sn --upperlimitmag --magnitude --dec --ra --y --x gnuastro-0.2.33-8a3b/tests/lib/0000755000175000017500000000000013004464727013114 500000000000000gnuastro-0.2.33-8a3b/tests/lib/versioncpp.cpp0000644000175000017500000000216312766612422015733 00000000000000/********************************************************************* A test program to get and use the version number of Gnuastro within C++. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include int main(void) { std::cout << "Gnuastro version is: " << GAL_GNUASTRO_VERSION << ".\n"; return EXIT_SUCCESS; } gnuastro-0.2.33-8a3b/tests/lib/multithread.c0000644000175000017500000001202713001632540015507 00000000000000/********************************************************************* A test program to multithreaded building using Gnuastro's helpers. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include "gnuastro/threads.h" /* The params structure will keep the input information for each thread. As you see below, we will actually be defining an array of these structures, one for each thread. The reason for this is that the function that spins off threads only passes one argument, so as that argument, we will be passing the pointer to this structure. You can easily add new elements to this structure to use in the threads function. */ struct params { size_t id; /* Id of this thread. */ size_t *indexs; /* Indexes of actions to be done in this thread. */ pthread_barrier_t *b; /* Pointer the barrier for all threads. */ }; /* Worker function on threads */ void * worker(void *inparam) { /* The first thing to do is to say what the input pointer actually is. */ struct params *prm=(struct params*)inparam; /* Now you can go onto do defining the function like any other function: first you define the variables and so on... */ size_t i; /* Go over the jobs indexed for this thread: */ for(i=0; prm->indexs[i] != GAL_THREADS_NON_THRD_INDEX; ++i) { /* The indexes of the actions will make it possible to point to whatever data structure or input you want. So in this test, we will just print the thread ID and action id. */ printf("thread %zu: %zu\n", prm->id, prm->indexs[i]); } /* Wait until all other threads finish. When there was only one thread, we explicitly set the pointer to the barrier structure to NULL, so only wait when a barrier is actually defined.*/ if(prm->b) pthread_barrier_wait(prm->b); /* Return the NULL pointer. */ return NULL; } /* This is the thread spinner function. */ int main(void) { int err; pthread_t t; /* All thread ids saved in this, not used. */ struct params *prm; size_t numbarriers; pthread_attr_t attr; pthread_barrier_t b; size_t i, *indexs, thrdcols; size_t numthreads=8, numactions=1000; /* Allocate the array of `param' structures. Note that in most cases, the number of threads will not be a constant like this simple case, it will be a variable passed to the thread-spinner. So we are using dynamic allocation for more general use as a tutorial. */ prm=malloc(numthreads*sizeof *prm); if(prm==NULL) { fprintf(stderr, "%zu bytes could not be allocated for prm.", numthreads*sizeof *prm); exit(EXIT_FAILURE); } /* Distribute the actions into the threads: */ gal_threads_dist_in_threads(numactions, numthreads, &indexs, &thrdcols); /* Do the job: when only one thread is necessary, there is no need to spin off one thread, just call the function directly (spinning off threads is expensive). This is for the generic thread spinner function, not this simple function where `numthreads' is a constant. */ if(numthreads==1) { prm[0].id=0; prm[0].b=NULL; prm[0].indexs=indexs; worker(&prm[0]); } else { /* Initialize the attributes. Note that this running thread (that spinns off the nt threads) is also a thread, so the number the barriers should be one more than the number of threads spinned off. */ numbarriers = (numactions Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include "gnuastro/array.h" #include "gnuastro/gnuastro.h" int main(void) { double *array; size_t i, size=6; /* Allocate the array, report an error if it wasn't allocated. */ array=malloc(size * sizeof *array); if(array==NULL) { fprintf(stderr, "%zu bytes for d.\n", size); exit(EXIT_FAILURE); } /* Print the version of Gnuastro being used: */ printf("Test of Gnuastro %s\n", GAL_GNUASTRO_VERSION); /* Fill in the test array and report its contents at the same time. */ printf("Input array: "); for(i=0;i # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=imgwarp img=convolve_spatial.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $img --output=homographic.fits \ --matrix="0.707106781,-0.707106781,0, 0.707106781, 0.707106781,0, 0.001,0.002,1" gnuastro-0.2.33-8a3b/tests/imgwarp/imgwarp_scale.sh0000755000175000017500000000232512771240364017111 00000000000000# Scale an image to 1/5th of its input scale. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=imgwarp img=convolve_spatial.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $img --matrix="0.2,0,0.4 0,0.2,0.4 0,0,1" gnuastro-0.2.33-8a3b/tests/imgstat/0000755000175000017500000000000013004464727014016 500000000000000gnuastro-0.2.33-8a3b/tests/imgstat/basicstats.sh0000755000175000017500000000231012771240367016433 00000000000000# Get basic image statistics. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=imgstat execname=../bin/$prog/ast$prog img=convolve_spatial_warped_noised.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $img --checkmode --mirrorquant=0.5 gnuastro-0.2.33-8a3b/tests/imgcrop/0000755000175000017500000000000013004464727014006 500000000000000gnuastro-0.2.33-8a3b/tests/imgcrop/cat.txt0000644000175000017500000000012612457430742015236 000000000000000 500.00 500.00 0.99917157 1.0008283 1 251.00 251.00 0.99958658 1.0004150 gnuastro-0.2.33-8a3b/tests/imgcrop/wcspolygon.sh0000755000175000017500000000256012771240362016471 00000000000000# Crop from a catalog using x and y coordinates in WCS mode. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=imgcrop img=mkprofcat*.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then exit 77; fi for fn in $img; do if [ ! -f $fn ]; then exit 77; fi; done # Actual test script # ================== $execname $img --wcsmode --zeroisnotblank --output=wcspolygon.fits \ --polygon=0.99980497,1.0001967:0.998378,1.0012267:0.9999766,1.0013217 gnuastro-0.2.33-8a3b/tests/imgcrop/imgoutpolygon.sh0000755000175000017500000000301612771240363017177 00000000000000# Crop an image based polygon from an image. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=imgcrop img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== # # The number of threads is one so if CFITSIO does is not configured to # enable multithreaded access to files, the tests pass. It is the # users choice to enable this feature. $execname $img $cat --imgmode --zeroisnotblank --outpolygon --keepblankcenter \ --polygon=209,50:436.76,151:475.64,438.2:210.6,454.04:121.4,289.88 \ --output=imgoutpolygon.fits gnuastro-0.2.33-8a3b/tests/imgcrop/imgpolygon.sh0000755000175000017500000000246212771240363016453 00000000000000# Crop an image based polygon from an image. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=imgcrop img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $img $cat --imgmode --zeroisnotblank --output=imgpolygon.fits \ --polygon=209,50:436.76,151:475.64,438.2:210.6,454.04:121.4,289.88 gnuastro-0.2.33-8a3b/tests/imgcrop/radec.sh0000755000175000017500000000245012771240362015341 00000000000000# Crop a box based on the --ra and --dec options. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=imgcrop img=mkprofcat*.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then exit 77; fi for fn in $img; do if [ ! -f $fn ]; then exit 77; fi; done # Actual test script # ================== $execname $img --ra=0.99917157 --dec=1.0008283 --wwidth=0.3 \ --output=imgcrop_radec.fits gnuastro-0.2.33-8a3b/tests/imgcrop/section.sh0000755000175000017500000000264612771240363015737 00000000000000# Crop a box based on a specified section. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=imgcrop img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== # # The number of threads is one so if CFITSIO does is not configured to # enable multithreaded access to files, the tests pass. It is the # users choice to enable this feature. $execname $img --section=-10:*+10,:250 --output=imgcrop_section.fits \ --numthreads=1 gnuastro-0.2.33-8a3b/tests/imgcrop/xcycnoblank.sh0000755000175000017500000000267112771240362016603 00000000000000# Crop a box based on --xc and --yc, with no blank pixels. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=imgcrop img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== # # The number of threads is one so if CFITSIO does is not configured to # enable multithreaded access to files, the tests pass. It is the # users choice to enable this feature. $execname $img --xc=500 --yc=500 --noblank --output=imgcrop_xcycnb.fits \ --numthreads=1 gnuastro-0.2.33-8a3b/tests/imgcrop/xcyc.sh0000755000175000017500000000261312771240363015233 00000000000000# Crop a box based on --xc and --yc. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=imgcrop img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== # # The number of threads is one so if CFITSIO does is not configured to # enable multithreaded access to files, the tests pass. It is the # users choice to enable this feature. $execname $img --xc=251 --yc=251 --output=imgcrop_xcyc.fits --numthreads=1 gnuastro-0.2.33-8a3b/tests/imgcrop/wcscat.sh0000755000175000017500000000275312771240363015556 00000000000000# Crop from a catalog using x and y coordinates in WCS mode. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=imgcrop img=mkprofcat*.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then exit 77; fi for fn in $img; do if [ ! -f $fn ]; then exit 77; fi; done # Actual test script # ================== # # The number of threads is one so if CFITSIO does is not configured to # enable multithreaded access to files, the tests pass. It is the # users choice to enable this feature. cat=$topsrc/tests/$prog/cat.txt $execname $cat $img --suffix=_wcscat.fits --zeroisnotblank --numthreads=1 gnuastro-0.2.33-8a3b/tests/imgcrop/imgcat.sh0000755000175000017500000000273212771240363015533 00000000000000# Crop from a catalog using x and y coordinates in Image mode. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=imgcrop img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== # # The number of threads is one so if CFITSIO does is not configured to # enable multithreaded access to files, the tests pass. It is the # users choice to enable this feature. cat=$topsrc/tests/$prog/cat.txt $execname $img $cat --imgmode --suffix=_imgcat.fits --zeroisnotblank \ --numthreads=1 gnuastro-0.2.33-8a3b/tests/header/0000755000175000017500000000000013004464727013576 500000000000000gnuastro-0.2.33-8a3b/tests/header/delete.sh0000755000175000017500000000226612771240364015324 00000000000000# Delete header information. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=header img=headertest.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $img --delete=ABSJUNK --delete=ABSJNK2 gnuastro-0.2.33-8a3b/tests/header/update.sh0000755000175000017500000000240612771240365015341 00000000000000# Update the full header information # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=header img=headertest.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $img --update=ABSJUNK,8.231,"An updated value.",s \ --update=ABSJNK2,1232,"Another updated value",kg gnuastro-0.2.33-8a3b/tests/header/print.sh0000755000175000017500000000223312771240364015210 00000000000000# Print the full header information # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=header img=headertest.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $img gnuastro-0.2.33-8a3b/tests/header/write.sh0000755000175000017500000000246412771240364015214 00000000000000# Write a junk header to a FITS file # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=header img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== cp $img headertest.fits $execname headertest.fits --write=ABSJUNK,10.92,"A Header Test.",m/s --date \ --write=ABSJNK2,2343fdsa,"Another absolute junk test!" gnuastro-0.2.33-8a3b/tests/cosmiccal/0000755000175000017500000000000013004464727014303 500000000000000gnuastro-0.2.33-8a3b/tests/cosmiccal/simpletest.sh0000755000175000017500000000207012771240370016746 00000000000000# A simple run of CosmicCalculator to check if it can run. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=cosmiccal execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # if [ ! -f $execname ]; then exit 77; fi # Actual test script # ================== $execname --redshift=2.5 gnuastro-0.2.33-8a3b/tests/convolve/0000755000175000017500000000000013004464727014201 500000000000000gnuastro-0.2.33-8a3b/tests/convolve/frequency.sh0000755000175000017500000000237712771240367016474 00000000000000# Convolve an image in the frequency domain. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). psf=psf.fits prog=convolve img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ] || [ ! -f $psf ]; then exit 77; fi # Actual test script # ================== $execname $img --kernel=$psf --frequency --output=convolve_frequency.fits gnuastro-0.2.33-8a3b/tests/convolve/spatial.sh0000755000175000017500000000237112771240370016114 00000000000000# Convolve an image in the spatial domain. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). psf=psf.fits prog=convolve img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ] || [ ! -f $psf ]; then exit 77; fi # Actual test script # ================== $execname $img --kernel=$psf --spatial --output=convolve_spatial.fits gnuastro-0.2.33-8a3b/tests/convertt/0000755000175000017500000000000013004464727014212 500000000000000gnuastro-0.2.33-8a3b/tests/convertt/fitstopdf.sh0000755000175000017500000000242612771240366016500 00000000000000# Convert a FITS image into an PDF file. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=convertt img=imgcrop_section.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). # # - Ghostscript was not present on the system. if [ ! -f $execname ] || [ ! -f $img ] || [ "x$hasghostscript" != "xyes" ]; then exit 77; fi # Actual test script # ================== $execname $img --output=pdf --log gnuastro-0.2.33-8a3b/tests/convertt/jpegtofits.sh0000755000175000017500000000241212771240365016646 00000000000000# Convert a FITS image into a one color JPEG file. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=convertt img=blankch.jpg execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). # # - libjpeg was not present on the system. if [ ! -f $execname ] || [ ! -f $img ] || [ "x$haslibjpeg" != "xyes" ]; then exit 77; fi # Actual test script # ================== $execname $img --output=fits gnuastro-0.2.33-8a3b/tests/convertt/fitstojpegcmyk.sh0000755000175000017500000000242612771240365017537 00000000000000# Convert a FITS image into a JPEG file. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). img=psf.fits prog=convertt execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). # # - libjpeg was not present on the system. if [ ! -f $execname ] || [ ! -f $img ] || [ "x$haslibjpeg" != "xyes" ]; then exit 77; fi # Actual test script # ================== $execname blank blank blank $img --output=f2jcmyk.jpg gnuastro-0.2.33-8a3b/tests/convertt/jpegtotxt.sh0000755000175000017500000000243512771240366016526 00000000000000# Convert a FITS image into a single channel JPEG image to text. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). img=psf.jpg prog=convertt execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). # # - libjpeg was not present on the system. if [ ! -f $execname ] || [ ! -f $img ] || [ "x$haslibjpeg" != "xyes" ]; then exit 77; fi # Actual test script # ================== $execname $img --output=jpegtotxt.txt gnuastro-0.2.33-8a3b/tests/convertt/blankch.sh0000755000175000017500000000244512771240365016100 00000000000000# Convert a FITS image into a one color JPEG file. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). img=psf.fits prog=convertt execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). # # - libjpeg was not present on the system. if [ ! -f $execname ] || [ ! -f $img ] || [ "x$haslibjpeg" != "xyes" ]; then exit 77; fi # Actual test script # ================== $execname blank $img blank --output=blankch.jpg --noinvert gnuastro-0.2.33-8a3b/tests/convertt/fitstojpeg.sh0000755000175000017500000000237312771240365016654 00000000000000# Convert a FITS image into a JPEG file. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). img=psf.fits prog=convertt execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). # # - libjpeg was not present on the system. if [ ! -f $execname ] || [ ! -f $img ] || [ "x$haslibjpeg" != "xyes" ]; then exit 77; fi # Actual test script # ================== $execname $img --output=jpg gnuastro-0.2.33-8a3b/tests/convertt/fitstotxt.sh0000755000175000017500000000225412771240365016544 00000000000000# Convert a FITS image into a text file. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). img=psf.fits prog=convertt execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $img --output=psf.txt gnuastro-0.2.33-8a3b/tests/arithmetic/0000755000175000017500000000000013004464727014477 500000000000000gnuastro-0.2.33-8a3b/tests/arithmetic/or.sh0000755000175000017500000000236012771240362015374 00000000000000# Choose two detected regions with the `or' operator # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=arithmetic execname=../bin/$prog/ast$prog img=convolve_spatial_noised_labeled.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $img 6 eq $img 3 eq or -h1 -h1 --output=or.fits gnuastro-0.2.33-8a3b/tests/arithmetic/where.sh0000755000175000017500000000240312771240361016063 00000000000000# Mask non-detected pixels in the image with the `where' operator. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=arithmetic execname=../bin/$prog/ast$prog img=convolve_spatial_noised_labeled.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $img $img 0 eq nan where -h0 -h1 --output=where.fits gnuastro-0.2.33-8a3b/tests/arithmetic/onlynumbers.sh0000755000175000017500000000204312771240361017326 00000000000000# Make an S/N image to test Arithmetic. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=arithmetic execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option). # if [ ! -f $execname ]; then exit 77; fi # Actual test script # ================== $execname -1 3.45 "*" gnuastro-0.2.33-8a3b/tests/arithmetic/snimage.sh0000755000175000017500000000240312771240361016374 00000000000000# Make an S/N image to test Arithmetic. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variabels (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=arithmetic execname=../bin/$prog/ast$prog img=convolve_spatial_noised_labeled.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ] || [ ! -f $img ]; then exit 77; fi # Actual test script # ================== $execname $img $img - $img / --hdu=0 --hdu=3 --hdu=4 \ --output=snimage.fits gnuastro-0.2.33-8a3b/doc/0000755000175000017500000000000013004464725011747 500000000000000gnuastro-0.2.33-8a3b/doc/gnuastro.info-30000644000175000017500000146404613004464701014557 00000000000000This is gnuastro.info, produced by makeinfo version 6.3 from gnuastro.texi. This book documents version 0.2.33-8a3b of the GNU Astronomy Utilities (Gnuastro). Gnuastro provides various programs and libraries for astronomical data manipulation and analysis. Copyright © 2015-2016 Free Software Foundation, Inc. Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled “GNU Free Documentation Licenseâ€. INFO-DIR-SECTION Astronomy START-INFO-DIR-ENTRY * Gnuastro: (gnuastro). GNU Astronomy Utilities. * help-gnuastro: (gnuastro)help-gnuastro mailing list. Getting help. * bug-gnuastro: (gnuastro)Report a bug. How to report bugs * ConvertType: (gnuastro)ConvertType. Convert different file types. * astconvertt: (gnuastro)Invoking astconvertt. Options to ConvertType. * Convolve: (gnuastro)Convolve. Convolve an input file with kernel. * astconvolve: (gnuastro)Invoking astconvolve. Options to Convolve. * CosmicCalculator: (gnuastro)CosmicCalculator. For cosmological params. * astcosmiccal: (gnuastro)Invoking astcosmiccal. Options to CosmicCalculator. * Header: (gnuastro)Header. Print and manipulate data header info. * astheader: (gnuastro)Invoking astheader. Options to Header. * ImageCrop: (gnuastro)ImageCrop. Crop region(s) from image(s). * astimgcrop: (gnuastro)Invoking astimgcrop. Options to ImageCrop. * Arithmetic: (gnuastro)Arithmetic. Arithmetic operations on pixels. * astarithmetic: (gnuastro)Invoking astarithmetic. Options to Arithmetic. * ImageStatistics: (gnuastro)ImageStatistics. Get image Statistics. * astimgstat: (gnuastro)Invoking astimgstat. Options to ImageStatistics. * ImageWarp: (gnuastro)ImageWarp. Warp an image to a new grid. * astimgwarp: (gnuastro)Invoking astimgwarp. Options to ImageWarp. * MakeCatalog: (gnuastro)MakeCatalog. Make a catalog from labeled image. * astmkcatalog: (gnuastro)Invoking astmkcatalog. Options to MakeCatalog. * MakeNoise: (gnuastro)MakeNoise. Make (add) noise to an image. * astmknoise: (gnuastro)Invoking astmkprof. Options to MakeNoise. * MakeProfiles: (gnuastro)MakeProfiles. Make mock profiles. * astmkprof: (gnuastro)Invoking astmkprof. Options to MakeProfiles. * NoiseChisel: (gnuastro)NoiseChisel. Detect signal in noise. * astnoisechisel: (gnuastro)Invoking astnoisechisel. Options to NoiseChisel. * SubtractSky: (gnuastro)SubtractSky. Find and subtract the sky value. * astsubtractsky: (gnuastro)Invoking astsubtractsky. Options to SubtractSky. * Table: (gnuastro)Table. Read and write FITS binary or ASCII tables. * asttable: (gnuastro)Invoking asttable. Options to Table. END-INFO-DIR-ENTRY  File: gnuastro.info, Node: Noise basics, Next: Invoking astmknoise, Prev: MakeNoise, Up: MakeNoise 8.2.1 Noise basics ------------------ Deep astronomical images, like those used in extragalactic studies seriously suffer from noise in the data. Generally speaking, the sources of noise in an astronomical image are photon counting noise and Instrumental noise which are discussed in detail below. We finish with a short introduction on how random numbers are generated and how you can determine the random number generator and seed value. * Menu: * Photon counting noise:: Poisson noise * Instrumental noise:: Readout, dark current and other sources. * Final noised pixel value:: How the final noised value is calculated. * Generating random numbers:: How random numbers are generated.  File: gnuastro.info, Node: Photon counting noise, Next: Instrumental noise, Prev: Noise basics, Up: Noise basics 8.2.1.1 Photon counting noise ............................. Thanks to the very accurate electronics used in today’s detectors, this type of noise is the main cause of concern for extra galactic studies. It can generally be associate with the counting error that is known to have a Poisson distribution. The Poisson distribution is about counting. But counting is a discrete operation with only positive values, for example we can’t count $3.2$ or $-2$ of anything. We only count $0$, $1$, $2$, $3$ and so on. Therefore the Poisson distribution is also a discrete distribution, only applying to whole positive integers. Let’s assume the mean value of counting something is known. In this case, the number of electrons that are produced by photons in the CCD. Let’s call this mean $\lambda$. Let’s take $k$ to represent the result of counting in one particular time we attempt to count. The probability density function of $k$ can be written as: $$f(k)={\lambda^k \over k!} e^{-\lambda},\quad k\in {0, 1, 2, 3, \dots }$$ Because the Poisson distribution is only applicable to positive values, it is by nature very skewed when $\lambda$ is near zero. One qualitative way to imagine it is that there simply aren’t enough integers smaller than $\lambda$, than there are larger integers. Therefore to accommodate all possibilities, it has to be skewed when $\lambda$ is small. But as $\lambda$ becomes larger and larger, the distribution becomes more and more symmetric. One very useful property of the Poisson distribution is that the mean value is also its variance. When $\lambda$ is very large, say $\lambda>1000$, then the normal (Gaussian) distribution, see *note PSF::, is an excellent approximation of the Poisson distribution with mean $\mu=\lambda$ and standard deviation $\sigma=\sqrt{\lambda}$. We see that the variance or dispersion of the distribution depends on the mean value, and when it is large it can be approximated with a Gaussian that only has one free parameter ($\mu=\lambda$ and $\sigma=\sqrt{\lambda}$) instead of two that it originally has. The astronomical objects after convolution with the PSF of the instrument, lie above a certain background flux. This background flux is defined to be the average flux of a region in the image that has absolutely no objects. The physical origin of this background value is the brightness of the atmosphere or possible stray light within the imaging instrument. It is thus an ideal definition, because in practice, what lies deep in the noise far lower than the detection limit is never known(1). However, in a real image, a relatively large number of very faint objects can been fully buried in the noise. These undetected objects will bias the background measurement to slightly larger values. The sky value is therefore defined to be the average of the undetected regions in the image, so in an ideal case where all the objects have been detected, the sky value and background value are the same. As longer wavelengths are used, the background value becomes more significant and also varies over a wide image field. Such variations are not currently implemented in MakeProfiles, but will be in the future. In a mock image, we have the luxury of setting the background value. In each pixel of the canvas of pixels, the flux is the sum of contributions from various sources after convolution. Let’s name this flux of the convolved sum of possibly overlapping objects, $I_{nn}$. $nn$ representing ‘no noise’. For now, let’s assume the background is constant and represented by $B$. In practice the background values are larger than $\sim1,000$ counts. Then the flux after adding noise is a random value taken from a Gaussian distribution with the following mean ($\mu$) and standard deviation ($\sigma$): $$\mu=B+I_{nn}, \quad \sigma=\sqrt{B+I_{nn}}$$ Since this type of noise is inherent in the objects we study, it is usually measured on the same scale as the astronomical objects, namely the magnitude system, see *note Flux Brightness and magnitude::. It is then internally converted to the flux scale for further processing. ---------- Footnotes ---------- (1) See the section on sky in Akhlaghi M., Ichikawa. T. 2015. Astrophysical Journal Supplement Series.  File: gnuastro.info, Node: Instrumental noise, Next: Final noised pixel value, Prev: Photon counting noise, Up: Noise basics 8.2.1.2 Instrumental noise .......................... While taking images with a camera, a dark current is fed to the pixels, the variation of the value of this dark current over the pixels, also adds to the final image noise. Another source of noise is the readout noise that is produced by the electronics in the CCD that attempt to digitize the voltage produced by the photo-electrons in the analog to digital converter. In deep extra-galactic studies these sources of noise are not as significant as the noise of the background sky. Let $C$ represent the combined standard deviation of all these sources of noise. If only this source of noise is present, the noised pixel value would be a random value chosen from a Gaussian distribution with $$\mu=I_{nn}, \quad \sigma=\sqrt{C^2+I_{nn}}$$ This type of noise is completely independent of the type of objects being studied, it is completely determined by the instrument. So the flux scale (and not magnitude scale) is most commonly used for this type of noise. In practice, this value is usually reported in ADUs not flux or electron counts. The gain value of the device can be used to convert between these two, see *note Flux Brightness and magnitude::.  File: gnuastro.info, Node: Final noised pixel value, Next: Generating random numbers, Prev: Instrumental noise, Up: Noise basics 8.2.1.3 Final noised pixel value ................................ Depending on the values you specify for $B$ and $C$ from the above, the final noised value for each pixel is a random value chosen from a Gaussian distribution with $$\mu=B+I_{nn}, \quad \sigma=\sqrt{C^2+B+I_{nn}}$$  File: gnuastro.info, Node: Generating random numbers, Prev: Final noised pixel value, Up: Noise basics 8.2.1.4 Generating random numbers ................................. As discussed above, to generate noise we need to make random samples of a particular distribution. So it is important to understand some general concepts regarding the generation of random numbers. For a very complete and nice introduction we strongly advise reading Donald Knuth’s “The art of computer programmingâ€, volume 2, chapter 3(1). Quoting from the GNU Scientific Library manual, “If you don’t own it, you should stop reading right now, run to the nearest bookstore, and buy itâ€(2)! Using only software, we can only produce what is called a psudo-random sequence of numbers. A true random number generator is a hardware (let’s assume we have made sure it has no systematic biases), for example throwing dice or flipping coins (which have remained from the ancient times). More modern hardware methods use atmospheric noise, thermal noise or other types of external electromagnetic or quantum phenomena. All psudo-random number generators (software) require a seed to be the basis of the generation. The advantage of having a seed is that if you specify the same seed for multiple runs, you will get an identical sequence of random numbers which allows you to reproduce the same final noised image. The programs in GNU Astronomy Utilities (for example MakeNoise or MakeProfiles) use the GNU Scientific Library (GSL) to generate random numbers. GSL allows the user to set the random number generator through environment variables, see *note Installation directory:: for an introduction to environment variables. In the chapter titled “Random Number Generation†they have fully explained the various random number generators that are available (there are a lot of them!). Through the two environment variables ‘GSL_RNG_TYPE’ and ‘GSL_RNG_SEED’ you can specify the generator and its seed respectively. If you don’t specify a value for ‘GSL_RNG_TYPE’, GSL will use its default random number generator type. The default type is sufficient for most general applications. If no value is given for the ‘GSL_RNG_SEED’ environment variable and you have asked Gnuastro to read the seed from the environment (through the ‘--envseed’ option), then GSL will use the default value of each generator to give identical outputs. If you don’t explicitly tell Gnuastro programs to read the seed value from the environment variable, then they will use the system time (accurate to within a microsecond) to generate (apparently random) seeds. In this manner, every time you run the program, you will get a different random number distribution. There are two ways you can specify values for these environment variables. You can call them on the same command-line for example: $ GSL_RNG_TYPE="taus" GSL_RNG_SEED=345 astmknoise input.fits In this manner the values will only be used for this particular execution of MakeNoise. To define them for the full period of your terminal session or script length, you can use the shell’s ‘export’ command (for a script remove the ‘$’ signs): $ export GSL_RNG_TYPE="taus" $ export GSL_RNG_SEED=345 The subsequent programs which use GSL’s random number generators will hence forth use these values in this session of the terminal you are running or while executing this script. In case you want set fixed values for these variables every time you use the GSL random number generator, you can add these two lines to your ‘.bashrc’ startup script(3), see *note Installation directory::. *NOTE:* If the two environment variables ‘GSL_RNG_TYPE’ and ‘GSL_RNG_SEED’ are defined, GSL will report them by default, even if you don’t use the ‘--envseed’ option. For example you can see the top few lines of the output of MakeProfiles: $ export GSL_RNG_TYPE="taus" $ export GSL_RNG_SEED=345 $ astmkprof catalog.txt --envseed GSL_RNG_TYPE=taus GSL_RNG_SEED=345 MakeProfiles started on AAA BBB DD EE:FF:GG HHH - 6 profiles read from catalog.txt 0.000236 seconds - Random number generator (RNG) type: taus - RNG seed for all profiles: 345 The first two output lines (showing the names of the environment variables) are printed by GSL before MakeProfiles actually starts generating random numbers. The Gnuastro programs will report the values they use independently, you should check them for the final values used. For example if ‘--envseed’ is not given, ‘GSL_RNG_SEED’ will not be used and the last line shown above will not be printed. In the case of MakeProfiles, each profile will get its own seed value. ---------- Footnotes ---------- (1) Knuth, Donald. 1998. The art of computer programming. Addison–Wesley. ISBN 0-201-89684-2 (2) For students, running to the library might be more affordable! (3) Don’t forget that if you are going to give your scripts (that use the GSL random number generator) to others you have to make sure you also tell them to set these environment variable separately. So for scripts, it is best to keep all such variable definitions within the script, even if they are within your ‘.bashrc’.  File: gnuastro.info, Node: Invoking astmknoise, Prev: Noise basics, Up: MakeNoise 8.2.2 Invoking MakeNoise ------------------------ MakeNoise will add noise to an existing image. The executable name is ‘astmknoise’ with the following general template $ astmknoise [OPTION ...] InputImage.fits One line examples: $ astmknoise --background=1000 --stdadd=20 mockimage.fits If actual processing is to be done, the input image is a mandatory argument. The full list of options common to all the programs in Gnuastro can be seen in *note Common options::. The output will have the same type as the input image, however the internal processing is done on a double precision floating point format. If the input values were integer types, then each floating point number will be rounded to the nearest integer away from zero. This might cause integer overflow if types with small ranges are used (for example images with a ‘BITPIX’ of ‘8’ which can only keep 256 values). This can be disabled with the ‘doubletype’ option. The header of the output FITS file keeps all the parameters that were influential in making it. This is done for future reproducibility. ‘-b’ ‘--background’ (‘=FLT’) The background pixel value for the image in units of magnitudes, see *note Photon counting noise:: and *note Flux Brightness and magnitude::. ‘-z’ ‘--zeropoint’ (‘=FLT’) The zeropoint magnitude used to convert the value of ‘--background’ (in units of magnitude) to flux, see *note Flux Brightness and magnitude::. ‘-s’ ‘--stdadd’ (‘=FLT’) The instrumental noise which is in units of flux, see *note Instrumental noise::. ‘-e’ ‘--envseed’ Use the ‘GSL_RNG_SEED’ environment variable for the seed used in the random number generator, see *note Generating random numbers::. With this option, the output image noise is always going to be identical (or reproducible). ‘-d’ ‘--doubletype’ Save the output in the double precision floating point format that was used internally. This option will be most useful if the input images were of integer types.  File: gnuastro.info, Node: High-level calculations, Next: Libraries, Prev: Modeling and fittings, Up: Top 9 High-level calculations ************************* After the reduction of raw data (for example with the programs in *note Image manipulation::) you will have reduced images/data ready for processing/analyzing (for example with the programs in *note Image analysis::). But the processed/analyzed data (or catalogs) are still not enough to derive any scientific result. Even higher-level analysis is still needed to convert the observed magnitudes, sizes or volumes into physical quantities that we associate with each catalog entry or detected object which is the purpose of the tools in this section. * Menu: * CosmicCalculator:: Calculate cosmological variables  File: gnuastro.info, Node: CosmicCalculator, Prev: High-level calculations, Up: High-level calculations 9.1 CosmicCalculator ==================== To derive higher-level information regarding our sources in extra-galactic astronomy, cosmological calculations are necessary. In Gnuastro, CosmicCalculator is in charge of such calculations. Before discussing how CosmicCalculator is called and operates (in *note Invoking astcosmiccal::), it is important to provide a rough but mostly self sufficient review of the basics and the equations used in the analysis. In *note Distance on a 2D curved space:: the basic idea of understanding distances in a curved and expanding 2D universe (which we can visualize) are reviewed. Having solidified the concepts there, in *note Extending distance concepts to 3D::, the formalism is extended to the 3D universe we are trying to study in our research. The focus here is obtaining a physical insight into these equations (mainly for the use in real observational studies). There are many books thoroughly deriving and proving all the equations with all possible initial conditions and assumptions for any abstract universe, interested readers can study those books. * Menu: * Distance on a 2D curved space:: Distances in 2D for simplicity * Extending distance concepts to 3D:: Going to 3D (our real universe). * Invoking astcosmiccal:: How to run CosmicCalculator  File: gnuastro.info, Node: Distance on a 2D curved space, Next: Extending distance concepts to 3D, Prev: CosmicCalculator, Up: CosmicCalculator 9.1.1 Distance on a 2D curved space ----------------------------------- The observations to date (for example the Plank 2013 results), have not measured the presence of a significant curvature in the universe. However to be generic (and allow its measurement if it does in fact exist), it is very important to create a framework that allows curvature. As 3D beings, it is impossible for us to mentally create (visualize) a picture of the curvature of a 3D volume in a 4D space. Hence, here we will assume a 2D surface and discuss distances on that 2D surface when it is flat, or when the 2D surface is curved (in a 3D space). Once the concepts have been created/visualized here, in *note Extending distance concepts to 3D::, we will extend them to the real 3D universe we live in and hope to study. To be more understandable (actively discuss from an observer’s point of view) let’s assume we have an imaginary 2D friend living on the 2D space (which _might_ be curved in 3D). So here we will be working with it in its efforts to analyze distances on its 2D universe. The start of the analysis might seem too mundane, but since it is impossible to imagine a 3D curved space, it is important to review all the very basic concepts thoroughly for an easy transition to a universe we cannot visualize any more (a curved 3D space in 4D). To start, let’s assume a static (not expanding or shrinking), flat 2D surface similar to *note Figure 9.1: flatplane. and that our 2D friend is observing its universe from point $A$. One of the most basic ways to parametrize this space is through the Cartesian coordinates ($x$, $y$). In *note Figure 9.1: flatplane, the basic axes of these two coordinates are plotted. An infinitesimal change in the direction of each axis is written as $dx$ and $dy$. For each point, the infinitesimal changes are parallel with the respective axes and are not shown for clarity. Another very useful way of parametrizing this space is through polar coordinates. For each point, we define a radius ($r$) and angle ($\phi$) from a fixed (but arbitrary) reference axis. In *note Figure 9.1: flatplane. the infinitesimal changes for each polar coordinate are plotted for a random point and a dashed circle is shown for all points with the same radius. [image src="gnuastro-figures/flatplane.png" text="../gnuastro-figures//flatplane.eps"] Figure 9.1: Two dimensional Cartesian and polar coordinates on a flat plane. Assuming a certain position, which can be parametrized as $(x,y)$, or $(r,\phi)$, a general infinitesimal change change in its position will place it in the coordinates $(x+dx,y+dy)$ and $(r+dr,\phi+d\phi)$. The distance (on the flat 2D surface) that is covered by this infinitesimal change in the static universe ($ds_s$, the subscript signifies the static nature of this universe) can be written as $$ds_s=dx^2+dy^2=dr^2+r^2d\phi^2$$The main question is this: how can our 2D friend incorporate the (possible) curvature in its universe when it is calculating distances? The universe it lives in might equally be a locally flat but globally curved surface like *note Figure 9.2: sphericalplane. The answer to this question but for a 3D being (us) is the whole purpose to this discussion. So here we want to give our 2D friend (and later, ourselves) the tools to measure distances if the space (that hosts the objects) is curved. *note Figure 9.2: sphericalplane. assumes a spherical shell with radius $R$ as the curved 2D plane for simplicity. The spherical shell is tangent to the 2D plane and only touches it at $A$. The result will be generalized afterwards. The first step in measuring the distance in a curved space is to imagine a third dimension along the $z$ axis as shown in *note Figure 9.2: sphericalplane. For simplicity, the $z$ axis is assumed to pass through the center of the spherical shell. Our imaginary 2D friend cannot visualize the third dimension or a curved 2D surface within it, so the remainder of this discussion is purely abstract for it (similar to us being unable to visualize a 3D curved space in 4D). But since we are 3D creatures, we have the advantage of visualizing the following steps. Fortunately our 2D friend knows our mathematics, so it can follow along with us. With the third axis added, a generic infinitesimal change over _the full_ 3D space corresponds to the distance: $$ds_s^2=dx^2+dy^2+dz^2=dr^2+r^2d\phi^2+dz^2.$$It is very important to recognize that this change of distance is for _any_ point in the 3D space, not just those changes that occur on the 2D spherical shell of *note Figure 9.2: sphericalplane. Recall that our 2D friend can only do measurements in the 2D spherical shell, not the full 3D space. So we have to constrain this general change to any change on the 2D spherical shell. To do that, let’s look at the arbitrary point $P$ on the 2D spherical shell. Its image ($P'$) on the flat plain is also displayed. From the dark triangle, we see that [image src="gnuastro-figures/sphericalplane.png" text="../gnuastro-figures//sphericalplane.eps"] Figure 9.2: 2D spherical plane (centered on $O$) and flat plane (gray) tangent to it at point $A$. $$\sin\theta={r\over R},\quad\cos\theta={R-z\over R}.$$These relations allow our 2D friend to find the value of $z$ (an abstract dimension for it) as a function of r (distance on a flat 2D plane, which it can visualize) and thus eliminate $z$. From $\sin^2\theta+\cos^2\theta=1$, we get $z^2-2Rz+r^2=0$ and solving for $z$, we find: $$z=R\left(1\pm\sqrt{1-{r^2\over R^2}}\right).$$The $\pm$ can be understood from *note Figure 9.2: sphericalplane.: For each $r$, there are two points on the sphere, one in the upper hemisphere and one in the lower hemisphere. An infinitesimal change in $r$, will create the following infinitesimal change in $z$: $$dz={\mp r\over R}\left(1\over \sqrt{1-{r^2/R^2}}\right)dr.$$Using the positive signed equation instead of $dz$ in the $ds_s^2$ equation above, we get: $$ds_s^2={dr^2\over 1-r^2/R^2}+r^2d\phi^2.$$ The derivation above was done for a spherical shell of radius $R$ as a curved 2D surface. To generalize it to any surface, we can define $K=1/R^2$ as the curvature parameter. Then the general infinitesimal change in a static universe can be written as: $$ds_s^2={dr^2\over 1-Kr^2}+r^2d\phi^2.$$Therefore, we see that a positive $K$ represents a real $R$ which signifies a closed 2D spherical shell like *note Figure 9.2: sphericalplane. When $K=0$, we have a flat plane (*note Figure 9.1: flatplane.) and a negative $K$ will correspond to an imaginary $R$. The latter two cases are open universes (where $r$ can extend to infinity). However, when $K>0$, we have a closed universe, where $r$ cannot become larger than $R$ as in *note Figure 9.2: sphericalplane. A very important issue that can be discussed now (while we are still in 2D and can actually visualize things) is that $\overrightarrow{r}$ is tangent to the curved space at the observer’s position. In other words, it is on the gray flat surface of *note Figure 9.2: sphericalplane, even when the universe if curved: $\overrightarrow{r}=P'-A$. Therefore for the point $P$ on a curved space, the raw coordinate $r$ is the distance to $P'$, not $P$. The distance to the point $P$ (at a specific coordinate $r$ on the flat plane) on the curved surface (thick line in *note Figure 9.2: sphericalplane.) is called the _proper distance_ and is displayed with $l$. For the specific example of *note Figure 9.2: sphericalplane, the proper distance can be calculated with: $l=R\theta$ ($\theta$ is in radians). using the $\sin\theta$ relation found above, we can find $l$ as a function of $r$: $$\theta=\sin^{-1}\left({r\over R}\right)\quad\rightarrow\quad l(r)=R\sin^{-1}\left({r\over R}\right)$$$R$ is just an arbitrary constant and can be directly found from $K$, so for cleaner equations, it is common practice to set $R=1$, which gives: $l(r)=\sin^{-1}r$. Also note that if $R=1$, then $l=\theta$. Generally, depending on the the curvature, in a _static_ universe the proper distance can be written as a function of the coordinate $r$ as (from now on we are assuming $R=1$): $$l(r)=\sin^{-1}(r)\quad(K>0),\quad\quad l(r)=r\quad(K=0),\quad\quad l(r)=\sinh^{-1}(r)\quad(K<0).$$With $l$, the infinitesimal change of distance can be written in a more simpler and abstract form of $$ds_s^2=dl^2+r^2d\phi^2.$$ Until now, we had assumed a static universe (not changing with time). But our observations so far appear to indicate that the universe is expanding (isn’t static). Since there is no reason to expect the observed expansion is unique to our particular position of the universe, we expect the universe to be expanding at all points with the same rate at the same time. Therefore, to add a time dependence to our distance measurements, we can simply add a multiplicative scaling factor, which is a function of time: $a(t)$. The functional form of $a(t)$ comes from the cosmology and the physics we assume for it: general relativity. With this scaling factor, the proper distance will also depend on time. As the universe expands (moves), the distance will also move to larger values. We thus define a distance measure, or coordinate, that is independent of time and thus doesn’t ‘move’ which we call the _comoving distance_ and display with $\chi$ such that: $l(r,t)=\chi(r)a(t)$. We thus shift the $r$ dependence of the proper distance we derived above for a static universe to the comoving distance: $$\chi(r)=\sin^{-1}(r)\quad(K>0),\quad\quad \chi(r)=r\quad(K=0),\quad\quad \chi(r)=\sinh^{-1}(r)\quad(K<0).$$ Therefore $\chi(r)$ is the proper distance of an object at a specific reference time: $t=t_r$ (the $r$ subscript signifies “referenceâ€) when $a(t_r)=1$. At any arbitrary moment ($t\neq{t_r}$) before or after $t_r$, the proper distance to the object can simply be scaled with $a(t)$. Measuring the change of distance in a time-dependent (expanding) universe will also involve the speed of the object changing positions. Hence, let’s assume that we are only thinking about the change in distance caused by something (light) moving at the speed of light. This speed is postulated as the only constant and frame-of-reference-independent speed in the universe, making our calculations easier, light is also the major source of information we receive from the universe, so this is a reasonable assumption for most extra-galactic studies. We can thus parametrize the change in distance as $$ds^2=c^2dt^2-a^2(t)ds_s^2 = c^2dt^2-a^2(t)(d\chi^2+r^2d\phi^2).$$  File: gnuastro.info, Node: Extending distance concepts to 3D, Next: Invoking astcosmiccal, Prev: Distance on a 2D curved space, Up: CosmicCalculator 9.1.2 Extending distance concepts to 3D --------------------------------------- The concepts of *note Distance on a 2D curved space:: are here extended to a 3D space that _might_ be curved in a 4D space. We can start with the generic infinitesimal distance in a static 3D universe, but this time not in spherical coordinates instead of polar coordinates. $\theta$ is shown in *note Figure 9.2: sphericalplane, but here we are 3D beings, positioned on $O$ (the center of the sphere) and the point $O$ is tangent to a 4D-sphere. In our 3D space, a generic infinitesimal displacement will have the distance: $$ds_s^2=dx^2+dy^2+dz^2=dr^2+r^2(d\theta^2+\sin^2{\theta}d\phi^2).$$Like our 2D friend before, we now have to assume an abstract dimension which we cannot visualize. Let’s call the fourth dimension $w$, then the general change in coordinates in the _full_ four dimensional space will be: $$ds_s^2=dr^2+r^2(d\theta^2+\sin^2{\theta}d\phi^2)+dw^2.$$But we can only work on a 3D curved space, so following exactly the same steps and conventions as our 2D friend, we arrive at: $$ds_s^2={dr^2\over 1-Kr^2}+r^2(d\theta^2+\sin^2{\theta}d\phi^2).$$In a non-static universe (with a scale factor a(t), the distance can be written as: $$ds^2=c^2dt^2-a^2(t)[d\chi^2+r^2(d\theta^2+\sin^2{\theta}d\phi^2)].$$  File: gnuastro.info, Node: Invoking astcosmiccal, Prev: Extending distance concepts to 3D, Up: CosmicCalculator 9.1.3 Invoking CosmicCalculator ------------------------------- CosmicCalculator will calculate cosmological variables based on the input parameters. The executable name is ‘astcosmiccal’ with the following general template $ astcosmiccal [OPTION...] ... One line examples: $ astcosmiccal --onlyvolume -z 0.8 $ astcosmiccal -l0.6964 -m0.3036 -z2.1 $ astcosmiccal --olambda=0.6964 --omatter=0.3036 --redshift=2.1 The input parameters can be given as command-line options or in the configuration files, see *note Configuration files::. For a definition of the different parameters, please see the sections prior to this. By default, all the cosmological calculations will be printed in the standard output (the command-line mainly) along with a short description and units. The options starting with ‘--only’ will only do that single desired calculation and only print the final number (in the same units as reported by default). These options are very useful when you want to call CosmicCalculator from a script. The resulting number can simply be put into a shell variable (for example ‘vol’) with the following line, which will allow you to use the value for any other subsequent operation. z=3.12 vol=$(astcosmiccal --redshift=$z --onlyvolume) In a script, this operation might be necessary for a very large number of objects (thousands of galaxies in a catalog for example). So the fact that all the other default calculations are ignored will also help you get to your result faster. If you just want to inspect the value of a variable, the description (which comes with units) might be more useful. In that case, the following command might be better. The other parameters will also be calculated, but they are so fast that you will not notice on modern computers. $ astcosmiccal --redshift=0.832 | grep volume The full list of options is shown and described below: ‘-z’ ‘--redshift’ (‘=FLT’) The redshift of interest. ‘-H’ ‘--H0’ (‘=FLT’) Current expansion rate (in km sec$^{-1}$ Mpc$^{-1}$). ‘-l’ ‘--olambda’ (‘=FLT’) Cosmological constant density divided by the critical density in the current Universe ($\Omega_{\Lambda,0}$). ‘-m’ ‘--omatter’ (‘=FLT’) Matter (including massive neutrinos) density divided by the critical density in the current Universe ($\Omega_{m,0}$). ‘-r’ ‘--oradiation’ (‘=FLT’) Radiation density divided by the critical density in the current Universe ($\Omega_{r,0}$). ‘-v’ ‘--onlyvolume’ Only print the comoving volume (in units of Mpc$^3$) until the desired redshift based on the input parameters. See explanations above for more on these types of options and how to effectively use them. ‘-d’ ‘--onlyabsmagconv’ Only print the conversion factor for apparent magnitude to absolute magnitude. Note that this is practically the distance modulus added with $-2.5\log{(1+z)}$ for the the desired redshift based on the input parameters. See explanations above for more on these types of options and how to effectively use them.  File: gnuastro.info, Node: Libraries, Next: Developing, Prev: High-level calculations, Up: Top 10 Libraries ************ Each program in Gnuastro that was discussed in the prior chapters (or any program in general) is a collection of functions that is compiled into one executable file which can communicate directly with the outside world. The outside world in this context is the operating system. By communication, we mean that control is directly passed to a program from the operating system with a (possible) set of inputs and after it is finished, the program will pass control back to the operating system. For programs written in C and C++, the unique ‘main’ function is in charge of this communication. Similar to a program, a library is also a collection of functions that is compiled into one executable file. However, unlike programs, libraries don’t have a ‘main’ function. Therefore they can’t communicate directly with the outside world. This gives you the chance to write your own ‘main’ function and call library functions from within it. After compiling your program into a binary executable, you just have to _link_ it to the library and you are ready to run (execute) your program. In this way, you can use Gnuastro at a much lower-level, and in combination with other libraries on your system, you can significantly boost your creativity. This chapter starts with a basic introduction to libraries and how you can use them in *note Review of library fundamentals::. The separate functions in the Gnuastro library are then introduced (classified by context) in *note Gnuastro library::. If you end up routinely using a fixed set of library functions, with a well-defined input and output, it will be much more beneficial if you define a program for the job. Therefore, in its *note Version controlled source::, Gnuastro comes with the *note The TEMPLATE program:: to easily define your own programs(s). * Menu: * Review of library fundamentals:: Guide on libraries and linking. * Gnuastro library:: Description of all library functions.  File: gnuastro.info, Node: Review of library fundamentals, Next: Gnuastro library, Prev: Libraries, Up: Libraries 10.1 Review of library fundamentals =================================== Gnuastro’s libraries are written in the C programming language. In *note Why C::, we have thoroughly discussed the reasons behind this choice. C was actually created to write Unix, thus understanding the way C works can greatly help in effectively using programs and libraries in all Unix-like operating systems. Therefore, in the following subsections some important aspects of C, as it relates to libraries (and thus programs that depend on them) on Unix are reviewed. First we will discuss header files in *note Headers:: and then go onto *note Linking::. This section finishes with *note Summary and example on libraries::. If you are already familiar with these concepts, please skip this section and go directly to *note Gnuastro library::. In theory, a full operating system (or any software) can be written as one function. Such a software would not need any headers or linking (that are discussed in the subsections below). However, writing that single function and maintaining it (adding new features, fixing bugs, documentation and etc) would be a programmer or scientist’s worst nightmare! Furthermore, all the hard work that went into creating it cannot be reused in other software: every other programmer or scientist would have to re-invent the wheel. The ultimate purpose behind libraries (which come with headers and have to be linked) is to address this problem and increase modularity: “the degree to which a system’s components may be separated and recombined†(from Wikipedia). The more modular the source code of a program or library, the easier maintaining it will be, and all the hard work that went into creating it can be reused for a wider range of problems. * Menu: * Headers:: Header files included in source. * Linking:: Linking the compiled source files into one. * Summary and example on libraries:: A summary and example on using libraries. * Automatic linking script:: Shell function for automatic linking.  File: gnuastro.info, Node: Headers, Next: Linking, Prev: Review of library fundamentals, Up: Review of library fundamentals 10.1.1 Headers -------------- C source code is read from top to bottom in the source file, therefore program components (for example variables, data structures and functions) should all be _defined_ or _declared_ closer to the top of the source file: before they are used. _Defining_ something in C or C++ is jargon for providing its full details. _Declaring_ it, on the other-hand, is jargon for only providing the minimum information needed for the compiler to pass it temporarily and fill in the detailed definition later. For a function, the _declaration_ only contains the inputs and their data-types along with the output’s type(1). The _definition_ adds to the declaration by including the exact details of what operations are done to the inputs to generate the output. As an example, take this simple summation function: double sum(double a, double b) { return a + b; } What you see above is the _definition_ of this function: it shows you (and the compiler) exactly what it does to the two ‘double’ type inputs and that the output also has a ‘double’ type. Note that a function’s internal operations are rarely so simple and short, it can be arbitrarily long and complicated. This unreasonably short and simple function was chosen here for ease of reading. The declaration for this function is: double sum(double a, double b); You can think of a function’s declaration as a building’s address in the city, and the definition as the building’s complete blueprints. When the compiler confronts a call to a function during its processing, it doesn’t need to know anything about how the inputs are processed to generate the output. Just as the postman doesn’t need to know the inner structure of a building when delivering the mail. The declaration (address) is enough. Therefore by _declaring_ the functions once at the start of the source files, we don’t have to worry about _defining_ them after they are used. Even for a simple real-world operation (not a simple summation like above!), you will soon need many functions (for example, some for reading/preparing the inputs, some for the processing, and some for preparing the output). Although it is technically possible, managing all the necessary functions in one file is not easy and is contrary to the modularity principle (see *note Review of library fundamentals::), for example the functions for preparing the input can be usable in your other projects with a different processing. Therefore, as we will see later (in *note Linking::), the functions don’t necessarily need to be defined in the source file where they are used. As long as their definitions are ultimately linked to the final executable, everything will be fine. For now, it is just important to remember that the functions that are called within one source file must be declared within the source file (declarations are mandatory), but not necessarily defined there. In the spirit of modularity, it is common to define contextually similar functions in one source file. For example, in Gnuastro, functions that calculate the median, mean and other statistical functions are defined in ‘lib/statistics.c’, while functions that deal directly with FITS files are defined in ‘lib/fits.c’. Keeping the definition of similar functions in a separate file greatly helps their management and modularity, but this fact alone doesn’t make things much easier for the caller’s source code: recall that while definitions are optional, declarations are mandatory. So if this was all, the caller would have to manually copy and paste (_include_) all the declarations from the various source files into the file they are working on now. To address this problem, programmers have adopted the header file convention: the header file of a source code contains all the declarations that a caller would need to be able to use any of its functions. For example, in Gnuastro, ‘lib/statistics.c’ (file containing function definitions) comes with ‘lib/gnuastro/statistics.h’ (only containing function declarations). The discussion above was mainly focused on functions, however, there are many more programming constructs such as pre-processor macros and data structures. Like functions, they also need to be known to the compiler when it confronts a call to them. So the header file also contains their definitions or declarations when they are necessary for the functions. Pre-processor macros (or macros for short) are replaced with their defined value by the pre-processor before compilation. Conventionally they are written only in capital letters to be easily recognized. It is just important to understand that the compiler doesn’t see the macros, it sees their fixed values. So when a header specifies macros you can do your programming without worrying about the actual values. The standard C types (for example ‘int’, or ‘float’) are very low-level and basic. We can collect multiple C types into a _structure_ for a higher-level way to keep and pass-along data. See *note FITS macros and data structures:: for some examples of macros and data structures. The contents in the header need to be _include_d into the caller’s source code with a special pre-processor command: ‘#include ’. As the name suggests, the _pre-processor_ goes through the source code prior to the processor (or compiler). One of its jobs is to include, or merge, the contents of files that are mentioned with this directive in the source code. Therefore the compiler sees a single entity containing the contents of the main file and all the included files. This allows you to include many (sometimes thousands of) declarations into your code with only one line. Since the headers are also installed with the library into your system, you don’t even need to keep a copy of them for each separate program, making things even more convenient. Try opening some of the ‘.c’ files in Gnuastro’s ‘lib/’ directory with a text editor to check out the include directives at the start of the file (after the copyright notice). Let’s take ‘lib/fits.c’ as an example. You will notice that Gnuastro’s header files (like ‘gnuastro/fits.h’) are indeed within this directory (the ‘fits.h’ file is in the ‘gnuastro/’ directory). You will notice that files like ‘stdio.h’, or ‘string.h’ are not in this directory (or anywhere within Gnuastro). On most systems the basic C header files (like ‘stdio.h’ and ‘string.h’ mentioned above) are located in ‘/usr/include/’(2). Your compiler is configured to automatically search that directory (and possibly others), so you don’t have to explicitly mention these directories. Go ahead, look into the ‘/usr/include’ directory and find ‘stdio.h’ for example. When the necessary header files are not in those specific libraries, the pre-processor can also search in places other than the current directory. You can specify those directories with this pre-processor option(3): ‘-I DIR’ “Add the directory ‘DIR’ to the list of directories to be searched for header files. Directories named by ’-I’ are searched before the standard system include directories. If the directory ‘DIR’ is a standard system include directory, the option is ignored to ensure that the default search order for system directories and the special treatment of system headers are not defeated...†(quoted from the GNU Compiler Collection manual). Note that the space between and the directory is optional and commonly not used. If the pre-processor can’t find the included files, it will abort with an error. In fact a common error when building programs that depend on a library is that the compiler doesn’t not know where a library’s header is (see *note Known issues::). So you have to manually tell the compiler where to look for the library’s headers with the ‘-I’ option. For a small software with one or two source files, this can be done manually (see *note Summary and example on libraries::). However, to enhance modularity, Gnuastro (and most other bin/libraries) contain many source files, so the compiler is invoked many times(4). This makes manual addition or modification of this option practically impossible. To solve this problem, in the GNU build system, there are conventional environment variables for the various kinds of compiler options (or flags). These environment variables are used in every call to the compiler (they can be empty). The environment variable used for the C Pre-Processor (or CPP) is ‘CPPFLAGS’. By giving ‘CPPFLAGS’ a value once, you can be sure that each call to the compiler will be affected. See *note Known issues:: for an example of how to set this variable at configure time. As described in *note Installation directory::, you can select the top installation directory of a software using the GNU build system, when you ‘./configure’ it. All the separate components will be put in their separate sub-directory under that, for example the programs, compiled libraries and library headers will go into ‘$prefix/bin’ (replace ‘$prefix’ with a directory), ‘$prefix/lib’, and ‘$prefix/include’ respectively. For enhanced modularity, libraries that contain diverse collections of functions (like GSL, WCSLIB, and Gnuastro), put their header files in a sub-directory unique to themselves. For example all Gnuastro’s header files are installed in ‘$prefix/include/gnuastro’. In your source code, you need to keep the library’s sub-directory when including the headers from such libraries, for example ‘#include ’(5). Not all libraries need to follow this convention, for example CFITSIO only has one header (‘fitsio.h’) which is directly installed in ‘$prefix/include’. ---------- Footnotes ---------- (1) Recall that in C, functions only have one output. (2) The ‘include/’ directory name is taken from the pre-processor’s ‘#include’ directive, which is also the motivation behind the ‘I’ in the ‘-I’ option to the pre-processor. (3) Try running Gnuastro’s ‘make’ and find the directories given to the compiler with the ‘-I’ option. (4) Nearly every command you see being executed after running ‘make’ is one call to the compiler. (5) the top ‘$prefix/include’ directory is usually known to the compiler  File: gnuastro.info, Node: Linking, Next: Summary and example on libraries, Prev: Headers, Up: Review of library fundamentals 10.1.2 Linking -------------- To enhance modularity, similar functions are defined in one source file (with a ‘.c’ suffix, see *note Headers:: for more). After running ‘make’, each human-readable, ‘.c’ file is translated (or compiled) into a computer-readable “object†file (ending with ‘.o’). Note that object files are also created when building programs, they aren’t particular to libraries. Try opening Gnuastro’s ‘lib/’ and ‘bin/progname/’ directories after running ‘make’ to see these object files(1). Afterwards, the object files are _linked_ together to create an executable program or a library. The object files contain the full definition of the functions in the respective ‘.c’ file along with a list of any other function (or generally “symbolâ€) that is referenced there. To get a list of those functions you can use the ‘nm’ program which is part of GNU Binutils. For example from the top Gnuastro directory, run: $ nm bin/arithmetic/arithmetic.o This will print a list of all the functions (more generally, ‘symbols’) that were called within ‘bin/arithmetic/arithmetic.c’ along with some further information (for example a ‘T’ in the second column shows that this function is actually defined here, ‘U’ says that it is undefined here). Try opening the ‘.c’ file to check some of these functions for your self. Run ‘info nm’ for more information. To recap, the _compiler_ created the separate object files mentioned above for each ‘.c’ file. The _linker_ will then combine all the symbols of the various object files (and libraries) into one program or library. In the case of Arithmetic (a program) the contents of the object files in ‘bin/arithmetic/’ are copied (and re-ordered) into one final executable file which we can run from the operating system. When the symbols (computer-readable function definitions in most cases) are copied into the output like this, we call the process _static_ linking. Let’s have a closer look at static linking: we’ll assume you have installed Gnuastro into the default ‘/usr/local/’ directory (see *note Installation directory::). If you tried the ‘nm’ command on one of Arithmetic’s object files above, then with the command below you can confirm that all the functions that were defined in the object files (had a ‘T’ in the second column) are also defined in the ‘astarithmetic’ executable: $ nm /usr/local/bin/astarithmetic But you will notice that there are still many undefined symbols (have a ‘U’ in the second column). One class of such functions are Gnuastro’s own library functions that start with ‘‘gal_’’: $ nm /usr/local/bin/astarithmetic | grep gal_ These undefined symbols (functions) will be linked to the executable every time you run arithmetic. Therefore they are known as dynamically _linked_ libraries (2). When the functions of a library need to be dynamically linked, the library is known as a shared library. As we saw above, static linking is done when the executable is being built. However, when a library is linked dynamically, its symbols are only checked with the available libraries at build time: they are not actually copied into the executable. Every time you run the program, the linker will be activated and will try to link the program to the installed library before it starts. If you want all the libraries to be statically linked to the executables, you have to tell Libtool (which Gnuastro uses for the linking) to disable shared libraries at configure time(3): $ configure --disable-shared Try configuring, statically building and installing Gnuastro with the command above. Then check the ‘gal_’ symbols in the installed Arithmetic executable like before. You will see that they are actually copied this time (have a ‘T’ in the second column). If the second column doesn’t convince you, look at the executable file size with the following command: $ ls -lh /usr/local/bin/astarithmetic It should be around 4.2 Megabytes with this static linking. If you configure and build Gnuastro again with shared libraries enabled (which is the default), you will notice that it is roughly 100 Kilobytes! This huge difference would have been very significant in the old days, but with the roughly Terabyte storages commonly in use today, it is negligible. Fortunately, output file size is not the only benefit of dynamic linking: since it links to the libraries at run-time (rather than build-time), you don’t have to re-build a higher-level program or library when an update comes for one of the lower-level libraries it depends on. You just install the new low-level library and it will automatically be used next time in your higher-level tools. To be fair, this also creates a few complications(4): • Reproducibility: Even though your high-level tool has the same version as before, with the updated library, you might not get the same results. • Broken links: if some functions have been changed or removed in the updated library, then the linker will abort with an error at run-time. Therefore you need to re-build your higher-level program or library. To see a list of all the shared libraries that are needed for a program or a shared library to run, you can use the GNU C library’s ‘ldd’(5) program, for example: $ ldd /usr/local/bin/astarithmetic Library file names start with a ‘lib’ and end with suffix depending on their type as described below. In between these two is the name of the library, for example ‘libgnuastro.a’ (Gnuastro’s static library) and ‘libgsl.so.0.0.0’ (GSL’s shared library). • A static library is known as an archive file and has a ‘.a’ suffix. A static library is not an executable file. • A shared library ends with a ‘.so.X.Y.Z’ suffix and is executable. The three numbers in the prefix are the version of the shared library. Shared library versions are defined to allow multiple versions of a shared library simultaneously on a system and to help detect possible updates in the library and programs that depend on it by the linker. It is very important to mention that this version number is different from from the software version number (see *note Version numbering::), so do not confuse the two. See the “Library interface versions†chapter of GNU Libtool for more. For each shared library, we also have two symbolic links ending with ‘.so.X’ and ‘.so’. They are automatically set by the installer, but you can change them (point them to another version of the library) when you have multiple versions on your system. For those libraries that use GNU Libtool (including Gnuastro and its dependencies), both static and dynamic libraries are built and installed in the ‘prefix/lib/’ directory (see *note Installation directory::). In this way other programs can make which ever kind of link that they want. To link with a library, the linker needs to know where to find the library. You do that with two separate options to the linker (see *note Summary and example on libraries:: for an example): ‘-L DIR’ Will tell the linker to look into ‘DIR’ for the libraries. For example ‘-L/usr/local/lib’, or ‘-L/home/yourname/.local/lib’. You can make multiple calls to this option, so the linker looks into several directories. Note that the space between and the directory is optional and commonly not used. ‘-lLIBRARY’ Specify the unique name of a library to be linked. As discussed above, library file names have fixed parts which must not be given to this option. So ‘-lgsl’ will guide the linker to either look for ‘libgsl.a’ or ‘libgsl.so’ (depending on the type of linking it is suppose to do). You can link many libraries by repeated calls to this option. *Very important: * The place of this option on the command line matters. This is often a source of confusion for beginners, so let’s assume you have asked the linker to link with library A using this option. As soon as the linker confronts this option, it looks into the list of the undefined symbols it has found until that point and does a search in library A for any of those symbols. If any pending undefined symbol is found in library A, it is used. After the search in undefined symbols is complete, the contents of library A are completely discarded from the linker’s memory. Therefore, if a later object file or library uses an unlinked symbol in library A, the linker will abort after it has finished its search in all the input libraries or object files. As an example, Gnuastro’s ‘gal_array_dlog10_array’ function depends on the ‘log10’ function of the C Math library (specified with ‘-lm’). So the proper way to link something that uses this function is ‘-lgnuastro -lm’. If instead, you give: ‘-lm -lgnuastro’ the linker will complain and abort. ---------- Footnotes ---------- (1) Gnuastro uses GNU Libtool for portable library creation. Libtool will also make a ‘.lo’ file for each ‘.c’ file when building libraries (‘.lo’ files are human-readable). (2) Do not confuse dynamically _linked_ libraries with dynamically _loaded_ libraries. The former (that is discussed here) are only loaded once at the program startup. However, the latter can be loaded anytime during the program’s execution, they are also known as plugins. (3) Libtool is very common and is commonly used. Therefore, you can use this option to configure on most programs using the GNU build system if you want static linking. (4) Both of these can be avoided by joining the mailing lists of the lower-level libraries and checking the changes in newer versions before installing them. Updates that result in such behaviors are generally heavily emphasized in the release notes. (5) If your operating system is not using the GNU C library, you might need another tool.  File: gnuastro.info, Node: Summary and example on libraries, Next: Automatic linking script, Prev: Linking, Up: Review of library fundamentals 10.1.3 Summary and example on libraries --------------------------------------- After the mostly abstract discussions of *note Headers:: and *note Linking::, we’ll give a small tutorial here. But before that, let’s recall the general steps of how your source code is prepared, compiled and linked to the libraries it depends on so you can run it: 1. The *pre-processor* includes the header (‘.h’) files into the function definition (‘.c’) files, expands pre-processor macros and generally prepares the human-readable source for compilation (reviewed in *note Headers::). 2. The *compiler* will translate (compile) the human-readable contents of each source (merged ‘.c’ and the ‘.h’ files, or generally the output of the pre-processor) into the computer-readable code of ‘.o’ files. 3. The *linker* will link the called function definitions from various compiled files to create one unified object. When the unified product has a ‘main’ function, this function is the product’s only entry point, enabling the operating system or user to directly interact with it, so the product is a program. When the product doesn’t have a ‘main’ function, the linker’s product is a library and its exported functions can be linked to other executables (it has many entry points). The GNU Compiler Collection (or GCC for short) will do all three steps. So as a first example, from Gnuastro’s source, go to ‘tests/lib/’. This directory contains the library tests, you can use these as some simple tutorials. For this demonstration, we will compile and run the ‘arraymanip.c’. This small program will call Gnuastro library for some simple operations on an array (open it and have a look). To compile this program, run this command inside the directory containing it. $ gcc arraymanip.c -lgnuastro -lm -o arraymanip The two ‘-lgnuastro’ and ‘-lm’ options (in this order) tell GCC to first link with the Gnuastro library and then with C’s math library. The ‘-o’ option is used to specify the name of the output executable, without it the output file name will be ‘a.out’ (on most OSs), independent of your input file name(s). If your top Gnuastro installation directory (let’s call it ‘$prefix’, see *note Installation directory::) is not recognized by GCC, you will get pre-processor errors for unknown header files. Once you fix it, you will get linker errors for undefined functions. To fix both, you should run GCC as follows: additionally telling it which directories it can find Gnuastro’s headers and compiled library (see *note Headers:: and *note Linking::): $ gcc -I$prefix/include -L$prefix/lib arraymanip.c -lgnuastro -lm \ -o arraymanip This single command has done all the pre-processor, compilation and linker operations. Therefore no intermediate files (object files in particular) were created, only a single output executable was created. You are now ready to run the program with: $ ./arraymanip The Gnuastro functions called by this program only needed to be linked with the C math library. But if your program needs WCS coordinate transformations, needs to read a FITS file, needs special math operations (which include its linear algebra operations), or you want it to run on multiple CPU threads, you also need to add these libraries in the call to GCC: ‘-lgnuastro -lwcs -lcfitsio -lgsl -lgslcblas -pthread -lm’. In *note Gnuastro library::, where each function is documented, it is mentioned which libraries (if any) must also be linked when you call a function. If you feel all these linkings can be confusing, please have a look at *note Automatic linking script::.  File: gnuastro.info, Node: Automatic linking script, Prev: Summary and example on libraries, Up: Review of library fundamentals 10.1.4 Automatic linking script ------------------------------- The number and order of libraries that are necessary for linking a program with Gnuastro library might be too confusing when you need to compile a small program for one particular job (with one source file). To solve this problem, please add these lines to your ‘~/.bashrc’ with a text editor and replace ‘PREFIX’ with Gnuastro’s installation directory (see *note Installation directory::). # Compile and correctly link Gnuastro related programs function gnuastro-gcc { libtool --mode=link gcc $1.c $2 PREFIX/lib/libgnuastro.la -o $1 } This tiny shell function uses GNU Libtool to find the necessary libraries to link against. Libtool uses the same libraries that were checked when you configured Gnuastro to link your program. So in the future, if Gnuastro’s prerequisite libraries change, you don’t have to worry. Afterwards, when you want to compile a C program that uses Gnuastro library (for example ‘myprog.c’), just run the following command from the directory which contains the source file: gnuastro-gcc myprog If your program needs to link with libraries other than those needed by Gnuastro, you can specify them as a second argument (within double quotes): gnuastro-gcc myprog "-lfirst -lsecond" If you also want to execute the compiled program without typing a second command, add ‘&& ./myprog’ to either of the lines above, like the example below. If your program can take arguments, then you can also include them afterwards. gnuastro-gcc myprog && ./myprog  File: gnuastro.info, Node: Gnuastro library, Prev: Review of library fundamentals, Up: Libraries 10.2 Gnuastro library ===================== Gnuastro library’s exported constructs (functions, macros, data structures, or global variables) are classified by context into multiple header files (see *note Headers::)(1). In this section, the functions in each header will be discussed under a separate sub-section, which includes the name of the header. Assuming a function declaration is in ‘headername.h’, you can include its declaration in your source code with: # include The names of all constructs are prefixed with ‘gal_headername_’ (or ‘GAL_HEADERNAME_’ for macros). The ‘gal_’ prefix stands for _G_NU _A_stronomy _L_ibrary. The ‘headername’ prefix is replaced by the header file name (without the ‘.h’) which contains the construct. All Gnuastro library functions are compiled into a single file which can be linked on the command-line with the ‘-lgnuastro’ option, (see *note Linking:: and *note Summary and example on libraries:: for an introduction). Gnuastro library is a high-level library which depends on lower level libraries for some operations (see *note Dependencies::). Therefore if at least one of Gnuastro’s functions in your program use functions from the dependencies, you will also need to link those dependencies after linking with Gnuastro. The outside libraries that need to be linked for such functions are mentioned following the function name. See *note Automatic linking script:: for a small shell function to worry about the libraries to link against and let you focus on your exciting science. *Libraries are still under heavy development: * Gnuastro was initially created to be a collection of command-line programs. However, as the programs and their the shared functions grew, internal (not installed) libraries were added. With the 0.2 release, the libraries are install able. Because of this history in these early phases, the libraries are not fully programmer friendly yet: they abort the program on an error, their naming and arguments are not fully uniform, or modular, and most of the interesting functions (that are currently only used within one program) are still internal to the program. During the next releases, Gnuastro’s library structure will undergo significant evolution to address all these problems. It will stabilize with the removal of this notice. Check the ‘NEWS’ file for interface changes. * Menu: * Installation information:: General information about the installation. * Array manipulation:: Functions for manipulating arrays. * Bounding box:: Finding the bounding box. * FITS files:: Working with FITS data. * Git wrappers:: Wrappers for functions in libgit2. * Linked lists:: Various types of linked lists. * Mesh grid for an image:: Breaking an image into a grid. * Polygons:: Working with the vertices of a polygon. * Qsort functions:: Helper functions for Qsort. * Spatial convolution:: Doing spatial convolution on an image * Statistical operations:: Functions for basic statistics. * Multithreaded programming:: Facilitating use of pthreads. * Text table into a C array:: Read an ASCII text table into a C array. * World Coordinate System:: Dealing with the world coordinate system. ---------- Footnotes ---------- (1) Within Gnuastro’s source, all installed ‘.h’ files in ‘lib/gnuastro/’ are accompanied by a ‘.c’ file in ‘/lib/’.  File: gnuastro.info, Node: Installation information, Next: Array manipulation, Prev: Gnuastro library, Up: Gnuastro library 10.2.1 Installation information (‘gnuastro.h’) ---------------------------------------------- The ‘gnuastro/gnuastro.h’ header contains information about the full Gnuastro installation on your system. Gnuastro developers should note that this is the only header that is not available within Gnuastro, it is only available to a Gnuastro library user _after_ installation. Within Gnuastro, ‘config.h’ (which is included in every Gnuastro ‘.c’ file, see *note Coding conventions::) should have more than enough information about the overall Gnuastro installation. -- Macro: GAL_GNUASTRO_VERSION This macro can be used as a string literal(1) containing the version of Gnuastro that is being used. See *note Version numbering:: for the version formats. For example: printf("Gnuastro version: %s\n", GAL_GNUASTRO_VERSION); or char *gnuastro_version=GAL_GNUASTRO_VERSION; -- Macro: GAL_GNUASTRO_HAVE_LIBGIT2 Libgit2 is an optional dependency of Gnuastro (see *note Optional dependencies::). When it is installed and detected at configure time, this macro will have a value of ‘1’. Otherwise, it will have a value of ‘0’. Gnuastro also comes with some wrappers to make it easier to use libgit2 (see *note Git wrappers::). -- Macro: GAL_GNUASTRO_HAVE_PTHREAD_BARRIER The POSIX threads standard define barriers as an optional requirement. Therefore, some operating systems choose to not include it. While installing Gnuastro, we check if your system has this construct and if so, we give this macro a value of ‘1’, otherwise it will have a value of ‘0’. see *note Implementation of pthread_barrier:: for more. ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: Array manipulation, Next: Bounding box, Prev: Installation information, Up: Gnuastro library 10.2.2 Array manipulation (‘array.h’) ------------------------------------- When working on arrays, certain operations are commonly necessary. It is very easy to write a loop for such operations, however such loops can unnecessarily make the code harder to write, read, and debug. So, it is much more cleaner if these operations are defined elsewhere. The declarations of these functions are available in ‘gnuastro/array.h’. In C, an array is a contiguous region of memory. So for most operations here, the dimentionality of the data is irrelevant, we just need the total size of the array. Please note that these functions are still very rudimentary, primarily intended for Gnuastro’s internal operations. In future releases, these functions will be updated to be more suitable for a generic library. -- Function: void gal_array_uchar_init_on_region (unsigned char ‘*in’, const unsigned char ‘v’, size_t ‘start’, size_t ‘s0’, size_t ‘s1’, size_t ‘is1’) Initialize a region of the array ‘in’ to the value ‘v’. The region is defined by the 1D index of the first pixel (‘start’) and its C array (opposite of FITS array) width (‘s0’) and height (‘s1’). The full C array width is defined by ‘is1’. -- Function: void gal_array_long_init (long ‘*in’, size_t ‘size’, const long ‘v’) Initialize the long type array ‘in’ with ‘size’ elements to the value ‘v’. -- Function: void gal_array_long_init_on_region (long ‘*in’, const long ‘v’, size_t ‘start’, size_t ‘s0’, size_t ‘s1’, size_t ‘is1’) Similar to ‘gal_array_uchar_init_on_region’ but for long type arrays. -- Function: void gal_array_uchar_copy (unsigned char ‘*in’, size_t ‘size’, unsigned char ‘**out’) Allocate space for and copy the input array ‘in’ with ‘size’ elements into an output array (‘out’). -- Function: void gal_array_float_copy (float ‘*in’, size_t ‘size’, float ‘**out’) Similar to ‘gal_array_uchar_copy’ but for the single precision floating point type. -- Function: void gal_array_float_copy_noalloc (float ‘*in’, size_t ‘size’, float ‘*out’) Similar to ‘gal_array_float_copy’ but the ‘out’ array must already be allocated. -- Function: void gal_array_fset_const (float ‘*in’, size_t ‘size’, float ‘a’) Set the input array ‘in’ with ‘size’ elements to the constant value ‘a’. -- Function: void gal_array_freplace_value (float ‘*in’, size_t ‘size’, float ‘from’, float ‘to’) Replace all elements with value ‘from’ to value ‘to’ in the ‘in’ array with ‘size’ elements. ‘from’ can be a NaN value, in this case, C’s ‘isnan’ function is used, not ‘==’. -- Function: void gal_array_freplace_nonnans (float ‘*in’, size_t ‘size’, float ‘to’) Replace any non-NaN value in the array ‘in’ with ‘size’ elements to the value ‘to’. -- Function: void gal_array_no_nans (float ‘*in’, size_t ‘*size’) Move all the non-NaN elements in the array ‘in’ to the start of the array so that the non-NaN elements are contiguous. This is useful for cases where you want to sort the data. Note that before this function, ‘size’ must point to the initial size of the array. After this function returns, size will point to the new size of the array, with only non-Nan elements. -- Function: void gal_array_no_nans_double (double ‘*in’, size_t ‘*size’) Similar to ‘gal_array_no_nans’ but for double types. -- Function: void gal_array_uchar_replace (unsigned char ‘*in’, size_t ‘size’, unsigned char ‘from’, unsigned char ‘to’) Replace all elements with value ‘from’ to value ‘to’ in the ‘in’ array with ‘size’ elements. -- Function: void gal_array_fmultip_const (float ‘*in’, size_t ‘size’, float ‘a’) Multiply all elements in the float array ‘in’ with size ‘size’ by the constant ‘a’. -- Function: void gal_array_fsum_const (float ‘*in’, size_t ‘size’, float ‘a’) Add all elements in the float array ‘in’ with size ‘size’ by the constant ‘a’. -- Function: float * gal_array_fsum_arrays (float ‘*in1’, float ‘*in2’, size_t ‘size’) Add the two arrays ‘in1’ and ‘in2’ and keep the result in a newly allocated array. The returned value is a pointer to that array. -- Function: void gal_array_dmultip_const (double ‘*in’, size_t ‘size’, double ‘a’) Multiply the double type array ‘in’ with ‘size’ elements with the constant ‘a’. -- Function: void gal_array_dmultip_arrays (double ‘*in1’, double ‘*in2’, size_t ‘size’) Multiply the two double type arrays ‘in1’ with ‘in2’ (both with ‘size’ elements) with each other and store the output in the first array. -- Function: void gal_array_ddivide_const (double ‘*in’, size_t ‘size’, double ‘a’) Divide the double type array ‘in’ with ‘size’ elements by the constant ‘a’. -- Function: void gal_array_dconst_divide (double ‘*in’, size_t ‘size’, double ‘a’) Divide the constant ‘a’ by the array ‘in’ with ‘size’ and store the result for each pixel in the array. -- Function: void gal_array_ddivide_arrays (double ‘*in1’, double ‘*in2’, size_t ‘size’) Divide each element of the two double array ‘in1’ by the elements in ‘in2’ (both with ‘size’ elements) and store the output in the first array. -- Function: void gal_array_dsum_const (double ‘*in’, size_t ‘size’, double ‘a’) Add the double type array ‘in’ with ‘size’ elements with the constant ‘a’. -- Function: void gal_array_dsum_arrays (double ‘*in1’, double ‘*in2’, size_t ‘size’) Add the two double type arrays ‘in1’ with ‘in2’ (both with ‘size’ elements) with each other and store the output in the first array. -- Function: void gal_array_dsubtract_const (double ‘*in’, size_t ‘size’, double ‘a’) Subtract the double type array ‘in’ with ‘size’ elements from the constant ‘a’. -- Function: void gal_array_dconst_subtract (double ‘*in’, size_t ‘size’, double ‘a’) Subtract the constant ‘a’ from the array ‘in’ with ‘size’ and store the result for each pixel in the array. -- Function: void gal_array_dsubtract_arrays (double ‘*in1’, double ‘*in2’, size_t ‘size’) Subtract each element of th the double type array ‘in2’ from ‘in1’ and put the result in the first array. -- Function: void gal_array_dpower_const (double ‘*in’, size_t ‘size’, double ‘a’) Each element in the intput array is taken to the power of of ‘a’ and stored in place. -- Function: void gal_array_dconst_power (double ‘*in’, size_t ‘size’, double ‘a’) The constant ‘a’ is taken to the power of each element in the intput array (‘in’) and stored in place. -- Function: void gal_array_dpower_arrays (double ‘*in1’, double ‘*in2’, size_t ‘size’) Each element in the first input array is taken to the power of the same element in the second array. -- Function: void gal_array_dlog_array (double ‘*in1’, size_t ‘size’) The natural logarithm of the input array is taken and stored in place. -- Function: void gal_array_dlog10_array (double ‘*in1’, size_t ‘size’) The base-10 logarithm of the input array is taken and stored in place. -- Function: void gal_array_dabs_array (double ‘*in1’, size_t ‘size’) Replace each element of the input array with its absolute value.  File: gnuastro.info, Node: Bounding box, Next: FITS files, Prev: Array manipulation, Up: Gnuastro library 10.2.3 Bounding box (‘box.h’) ----------------------------- Functions related to reporting a the bounding box of certain inputs are declared in ‘gnuastro/box.h’. All coordinates in this header are in the FITS format (first axis is the horizontal and the second axis is vertical). -- Function: void gal_box_ellipse_in_box (double ‘A’, double ‘B’, double ‘theta_rad’, long ‘*width’) Any ellipse can be enclosed into a rectangular box. The purpose of this function is to give the height and width of that box. ‘A’ is the ellipse major axis, ‘B’ is the minor axis, ‘theta_rad’ is the position angle in radians. The ‘width’ array will contain the output size in long integer type. ‘width[0]’, and ‘width[1]’ are the number of pixels along the first and second FITS axis. -- Function: void gal_box_border_from_center (double ‘xc’, double ‘yc’, long ‘*width’, long ‘*fpixel’, long ‘*lpixel’) Given the center (‘xc’ and ‘yc’) and width (two element array) of a box, return the coordinates of the first ‘fpixel’ and last ‘lpixel’ pixels (both are two element arrays. -- Function: int gal_box_overlap (long ‘*naxes’, long ‘*fpixel_i’, long ‘*lpixel_i’, long ‘*fpixel_o’, long ‘*lpixel_o’) We have an image of size ‘naxes’ and want to get the overlap of the image with a box. This function will return 1 if there is an overlap and 0 if there isn’t. The input and output box are specified by their first and last pixels. When there is an overlap, the coordinates of the first and last pixels of the overlap will be put in ‘fpixel_o’ and ‘lpixel_o’.  File: gnuastro.info, Node: FITS files, Next: Git wrappers, Prev: Bounding box, Up: Gnuastro library 10.2.4 FITS files (‘fits.h’) ---------------------------- The FITS format is the most common format to store data (images and tables) in astronomy. The CFITSIO library already provides a very good low-level set of functions for manipulating FITS data. Some CFITSIO operations (with well-defined inputs and outputs) are commonly needed in a special order. Therefore Gnuastro comes with the macros, data structures and functions introduced in this section. These functions are actually wrappers around CFITSIO functions for a higher-level (easier) access to FITS data. So if you feel these functions don’t exactly do what you want, we strongly recommend reading the CFITSIO manual to use it directly. All the functions and macros introduced in this section are declared in ‘gnuastro/fits.h’. When you include this header, you are also including CFITSIO’s ‘fitsio.h’ header. So you don’t need to explicitly include ‘fitsio.h’ anymore and can freely use any of its macros or functions in your code along with those discussed here. In *note CFITSIO datatype:: we first have a look at the way data types are referenced in CFITSIO (and thus Gnuastro). *note FITS macros and data structures:: defines the macros and data structures that can be used in functions for a unified format. This subsection finished with *note FITS functions::, which introduce the different Gnuastro functions available. * Menu: * CFITSIO datatype:: Addressing different types of data * FITS macros and data structures:: Gnuastro FITS related macros and structures. * FITS functions:: Functions to work on FITS data.  File: gnuastro.info, Node: CFITSIO datatype, Next: FITS macros and data structures, Prev: FITS files, Up: FITS files 10.2.4.1 CFITSIO ‘datatype’ ........................... Data can have multiple types: standards to convert a number of bits (which can only have values of 0 and 1) to different number formats (for example integer or floating point numbers). To store data, the FITS standard defines two major formats: images and tables. An image has a single type for all its data elements (a pixel in a 2D image). A table has a single type for every one of its columns. In both cases, the FITS header stores this information. All the FITS data types correspond to C types (for example ‘short’, ‘int’, ‘float’, or ‘long’). In images, the ‘BITPIX’ header keyword specifies the type of data in each pixel. Within CFITSIO, the different acceptable values of ‘BITPIX’ are stored as macros ending with ‘_IMG’. For example ‘BYTE_IMG’, or ‘DOUBLE_IMG’. See Section 4.1, “CFITSIO Definitionsâ€, in the CFITSIO manual for the recognized CFITSIO types and their macros. However, the FITS standard also accepts tables: each column in a FITS table has a unique ‘TFORM’ header keyword which specifies the type of data in that column. The variety of types in a FITS table can be much larger than an image and thus the standard for identifying them differs. To address these different formats of identifying the type in a uniform infra-structure, CFITSIO identifies a general collection of macros referring to types which can be internally used in all cases (images and tables). Thus in CFITSIO, the variable name ‘datatype’ when we are referring to this general collection of types. The image types are a subset of the table column types, so each acceptable ‘datatype’ corresponds to one of the table types. The macros for each recognized CFITSIO ‘datatype’ start with ‘T’, for example ‘TBYTE’, ‘TDOUBLE’. In CFITSIO (and thus here in Gnuastro), the ‘datatype’ is most commonly used, so this variable only accepts one of the accepted ‘T’ macros. When the ‘BITPIX’ value is desired (as input or output), the variable is called ‘bitpix’. In Gnuastro, the functions ‘gal_fits_bitpix_to_datatype’ and ‘gal_fits_tform_to_datatype’ are provided to convert ‘bitpix’ and ‘tform’ values to ‘datatype’. *CFITSIO integer types:* CFITSIO does not use the standard fixed integer size types of ‘stdint.h’! It uses the subjective ‘short’, ‘int’ and ‘long’ variables which can differ in size from system to system. For example, the FITS standard defines ‘LONG_IMG’ as a 32bit signed integer type, but CFITSIO converts it to a local ‘long’ which is 64 bits on a modern (64 bit) machine. To use CFITSIO, we had to adopt the same convention in Gnuastro. This issue can cause confusions, so be careful!  File: gnuastro.info, Node: FITS macros and data structures, Next: FITS functions, Prev: CFITSIO datatype, Up: FITS files 10.2.4.2 FITS macros and data structures ........................................ To facilitate handling of fixed/standard values and store, or pass multiple related variables in your programs, Gnuastro defines the following FITS related macros and data structures, see *note Headers:: for a more detailed discussion. -- Macro: GAL_FITS_STRING_BLANK -- Macro: GAL_FITS_BYTE_BLANK -- Macro: GAL_FITS_LOGICAL_BLANK -- Macro: GAL_FITS_SHORT_BLANK -- Macro: GAL_FITS_LONG_BLANK -- Macro: GAL_FITS_LLONG_BLANK -- Macro: GAL_FITS_FLOAT_BLANK -- Macro: GAL_FITS_DOUBLE_BLANK -- Macro: GAL_FITS_INT_BLANK -- Macro: GAL_FITS_SBYTE_BLANK -- Macro: GAL_FITS_UINT_BLANK -- Macro: GAL_FITS_USHORT_BLANK -- Macro: GAL_FITS_ULONG_BLANK These macros keep Gnuastro’s blank value constant for all the recognized datatypes in CFITSIO (see *note Blank pixels:: for a discussion on blank values). The values for the different types are mostly the lowest or highest possible value for that type (for unsigned types and 8-bit types, the maximum is used). So you can safely ignore the actual value and simply use these values to check. See explanation under the *note CFITSIO datatype:: function for more on types of data in FITS. The ‘float’ and ‘double’ types use the IEEE NaN values and for string it is a ‘NULL’ pointer. By definition, a NaN value fails in every condition check, so a NaN value is not equal to itself and the check ‘variable==GAL_FITS_FLOAT_BLANK’ will fail even if the value in ‘variable’ is NaN. Therefore, to check for blank values in floating point types be careful to use C’s ‘isnan’ function. -- Structure: gal_fits_key Structure for reading FITS header keywords. This structure will keep the name and value of one keyword. The value will be stored in the element corresponding to the type of the value. When multiple keywords must be read, you can define an array of this structure, for example the following declaration will allocate an array of five keywords to be read. struct gal_fits_key keys[5]; The names of the keywords can then be stored separately in the array and this expression will store the values in each element. gal_fits_read_keywords("filename.fits", hdu, gal_fits_key, 5); The FITS standard defines a maximum length for the value of keyword, so the space for the ‘str’ element is statically allocated (‘FLEN_VALUE’, which is defined in CFITSIO). So if the string value is necessary where ‘gal_fits_key’ is no longer available, then you have to allocate space dynamically and copy the string there. struct gal_fits_key { int status; /* CFITSIO status. */ char *keyname; /* Name of keyword. */ int datatype; /* Type of keyword value. */ char str[FLEN_VALUE]; /* String value. */ unsigned char u; /* Byte value. */ short s; /* Short integer value. */ long l; /* Long integer value. */ LONGLONG L; /* Long Long value. */ float f; /* Float value. */ double d; /* Double value. */ }; -- Structure: gal_fits_key_ll Structure for writing FITS keywords. This structure is used for one keyword. However, with the ‘next’ element, it can link to another keyword thus creating a linked list to add any number of keywords easily and at any step during your program. Adding new keywords doesn’t have to be done manually, the ‘gal_fits_add_to_key_ll’ and ‘gal_fits_add_to_key_ll_end’ will add new keywords for you to the start or end of the list to make a last-in-first-out or first-in-last-out list. See *note Linked lists:: for more on the nature of linked lists and more similar structures. struct gal_fits_key_ll { int kfree; /* ==1, free keyword name. */ int vfree; /* ==1, free keyword value. */ int cfree; /* ==1, free comment. */ int datatype; /* Keyword value datatype. */ char *keyname; /* Keyword Name. */ void *value; /* Keyword value. */ char *comment; /* Keyword comment. */ char *unit; /* Keyword unit. */ struct gal_fits_key_ll *next; /* Pointer next keyword. */ };  File: gnuastro.info, Node: FITS functions, Prev: FITS macros and data structures, Up: FITS files 10.2.4.3 FITS functions ....................... Gnuastro provides the following functions to deal with FITS data related operations. FITS data can have a variety of types, see *note CFITSIO datatype:: for a discussion on this, in particular the integer variables named ‘datatype’, ‘bitpix’, and ‘tform’. See *note FITS macros and data structures:: for the structure and macro definitions. -- Function: void gal_fits_io_error (int ‘status’, char ‘*message’) Report the input or output error as a string and print it along with a short statement that an error in CFITSIO occurred. All CFITSIO functions will change the value of ‘status’ if an error occurs. This function will print the CFITSIO error string from the value of ‘status’ followed by an optional ‘message’ that you can add to it. If the value of ‘message’ is ‘NULL’, then a default message will be printed. -- Function: int gal_fits_name_is_fits (char ‘*name’) Return ‘1’ if the string pointed by ‘name’ is a standard FITS filename (or more generally: can be read by CFITSIO) and ‘0’ if it isn’t. See *note Arguments:: for the standard FITS filenames. -- Function: int gal_fits_suffix_is_fits (char ‘*suffix’) Return ‘1’ if the string pointed by ‘suffix’ is a standard FITS suffix (or more generally: can be read by CFITSIO) and ‘0’ if it isn’t. ‘suffix’ can contain a dot or not (for example both ‘.fits’ and ‘fits’ will return ‘1’. See *note Arguments:: for the standard FITS filenames. -- Function: int gal_fits_bitpix_to_datatype (int ‘bitpix’) Return the datatype corresponding to the given ‘bitpix’ (value to the ‘BITPIX’ header keyword) in a FITS image. -- Function: int gal_fits_tform_to_datatype (char ‘tform’) Return the datatype corresponding to the given ‘tform’ character of a FITS table column: value to the ‘TFORM’ header keyword for the column. Note that in the FITS standard, ‘TFORM’ values are characters. -- Function: void gal_fits_img_bitpix_size (fitsfile ‘*fptr’, int ‘*bitpix’, long ‘*naxes’) Return the datatype (in FITS ‘BITPIX’ format) and image size of a FITS HDU specified with the ‘fitsfile’ pointer (defined in CFITSIO). So the HDU must have been already opened. If the number of dimensions is not 2, this function will return an error and abort. -- Function: void * gal_fits_datatype_blank (int ‘datatype’) Allocate the necessary space and put the blank value of type ‘datatype’ in it. Finally, return the pointer to the allocated space. This pointer is commonly necessary when calling CFITSIO read functions as ‘nulval’. See *note CFITSIO datatype::. -- Function: void * gal_fits_datatype_alloc (size_t ‘size’, int ‘datatype’) Allocate an array of ‘size’ elements of type ‘datatype’. See *note CFITSIO datatype::. -- Function: size_t gal_fits_datatype_size (int ‘datatype’) Return the size (in bytes) of the type specified by ‘datatype’, see *note CFITSIO datatype::. -- Function: void gal_fits_blank_to_value (void ‘*array’, int ‘datatype’, size_t ‘size’, void ‘*value’) Convert the blank values in ‘array’ (with ‘size’ elements) into the value pointed by ‘value’. -- Function: void gal_fits_change_type (void ‘*in’, int ‘inbitpix’, size_t ‘size’, int ‘anyblank’, void ‘**out’, int ‘outbitpix’) Convert the ‘in’ array (with ‘inbitpix’ type) into an array of type ‘outbitpix’ that is pointed by ‘out’. Space will be allocated for the output array within this function. -- Function: void gal_fits_num_hdus (char ‘*filename’, int ‘*numhdu’) Find the number of HDUs in ‘filename’ and store it in the space pointed to by ‘numhdu’. -- Function: void gal_fits_read_hdu (char ‘*filename’, char ‘*hdu’, unsigned char ‘img0_tab1’, fitsfile ‘**outfptr’) Open the HDU ‘hdu’ (a string) of the ‘filename’ FITS file into the ‘outfptr’. See ‘--hdu’ option in *note Input output:: for the accepted HDU formats. -- Function: void gal_fits_read_keywords (char ‘*filename’, char ‘*hdu’, struct gal_fits_key ‘*keys’, size_t ‘num’) Read ‘num’ keywords (identified in the ‘keys’ array) in the ‘hdu’ HDU of ‘filename’. See *note FITS macros and data structures:: for the definition of ‘gal_fits_key’ and its recommended usage with this function. CFITSIO will look for the next keyword starting from the last keyword found. Therefore, it is most efficient to specify the keywords in the same order as they appear in the desired HDU. -- Function: void gal_fits_add_to_key_ll (struct gal_fits_key_ll ‘**list’, int ‘datatype’, char ‘*keyname’, int ‘kfree’, void ‘*value’, int ‘vfree’, char ‘*comment’, int ‘cfree’, char ‘*unit’) Add an element to the top of the ‘gal_fits_key_ll’ linked list for writing keywords. This structure (or linked list) is used to write FITS keywords and is fully described in *note FITS macros and data structures::. Each variable also has the same name as the structure element that is described there. Assuming all the keywords were added with this function, you will have a last-in-first-out list: as the the name suggests, the last keyword you add to the list will be the first one that gets popped out and thus written in the FITS file header. -- Function: void gal_fits_add_to_key_ll_end (struct gal_fits_key_ll ‘**list’, int ‘datatype’, char ‘*keyname’, int ‘kfree’, void ‘*value’, int ‘vfree’, char ‘*comment’, int ‘cfree’, char ‘*unit’) Similar to ‘gal_fits_add_to_key_ll’, except the keyword is added to the end of the list, creating a first-in-first-out list. Therefore the order the keywords are written to the FITS header is the same as the order you have called this function. -- Function: void gal_fits_file_name_in_keywords (char ‘*keynamebase’, char ‘*filename’, struct gal_fits_key_ll ‘**list’) Put a filename into the ‘gal_fits_key_ll’ list to later write into a HDU header. The FITS standard sets a maximum length for the value of a keyword. This creates problems with file names (including directories), because they can become very long. Therefore, when the filename is longer than the maximum length of a FITS keyword value, this function will break it into several keywords. The ‘keynamebase’ string will be appended with a ‘_N’ (N>0) and used as the keyword name. -- Function: void gal_fits_add_wcs_to_header (fitsfile ‘*fptr’, char ‘*wcsheader’, int ‘nkeyrec’) Add the WCS information into the header of the HDU pointed to by ‘fptr’. The WCS information must already be converted into a long string with the FITS conventions. To help in identifying the WCS information, a few blank lines and a title will be added on top. -- Function: void gal_fits_update_keys (fitsfile ‘*fptr’, struct gal_fits_key_ll ‘**keylist’) Given the an opened FITS HDU (pointed to by ‘fptr’), this function will write, or update, all the keywords given in ‘keylist’. See *note FITS macros and data structures:: for more information on the ‘gal_fits_key_ll’ structure or linked list. -- Function: void gal_fits_write_keys_version (fitsfile ‘*fptr’, struct gal_fits_key_ll ‘*headers’, char ‘*spack_string’) Write or update (all the) keyword(s) in ‘headers’ into the FITS pointer, but also the date, name of your program (‘spack_string’), along with the versions of Gnuastro, CFITSIO, WCSLIB (when available) into the header, see *note Output headers::. Since the data processing depends on the versions of the libraries you have used, it is strongly recommended to include this information in every FITS output. See *note FITS macros and data structures:: for more information on the ‘gal_fits_key_ll’ structure or linked list. -- Function: void gal_fits_read_wcs_from_pointer (fitsfile ‘*fptr’, int ‘*nwcs’, struct wcsprm ‘**wcs’, size_t ‘hstartwcs’, size_t ‘hendwcs’) Read the WCSLIB WCS structure (‘wcs’, and ‘nwcs’ the number of WCS structures) from the FITS pointer ‘fptr’. In some cases, it might be necessary to only consider header keywords between a certain range. You can define the range of keywords to look for WCS information with the ‘hstartwcs’ and ‘hendwcs’ arguments. The range of header keywords will only be considered when the value of ‘hstartwcs’ is less than ‘hendwcs’, so if you don’t want to limit the range, set both values to 0. After you have finished using the WCS structure, use ‘wcsvfree(&nwcs,&wcs);’ to free it. *WCSLIB is not thread-safe: * WCSLIB’s ‘wcspih’ function is used by to read the FITS keywords into WCSLIB’s internal WCS structures. Unfortunately this function is not thread-safe. Therefore, be sure to call that function (or Gnuastro’s ‘gal_fits_read_wcs_from_pointer’ and ‘gal_fits_read_wcs’) before spinning off threads, see *note Multithreaded programming::. -- Function: void gal_fits_read_wcs (char ‘*filename’, char ‘*hdu’, size_t ‘hstartwcs’, size_t ‘hendwcs’, int ‘*nwcs’, struct wcsprm ‘**wcs’) Read the WCSLIB WCS structure (‘wcs’ and ‘nwcs’ the number of WCS structures) from a FITS file (‘hdu’ in ‘filename’). This is basically just a wrapper around the ‘gal_fits_read_wcs_from_pointer’ function, see that function for more. -- Function: int gal_fits_hdu_to_array (char ‘*filename’, char ‘*hdu’, int ‘*bitpix’, void ‘**array’, size_t ‘*s0’, size_t ‘*s1’) Read the FITS image (in the ‘hdu’ extension of ‘filename’). The image array will be stored in ‘array’ and the number of pixels in the first and second C axis will be stored in ‘s0’ and ‘s1’. The type of the array will be kept in ‘bitpix’. See ‘--hdu’ in *note Input output:: for the acceptable formats of ‘hdu’. -- Function: void gal_fits_array_to_file (char ‘*filename’, char ‘*extname’, int ‘bitpix’, void ‘*array’, size_t ‘s0’, size_t ‘s1’, int ‘anyblank’, struct wcsprm ‘*wcs’, struct gal_fits_key_ll ‘*headers’, char ‘*spack_string’) Write the array ‘array’ (with sizes ‘s0’ and ‘s1’, type ‘bitpix’, and WCS structure ‘wcs’) into the FITS file ‘filename’ and extension name ‘extname’. If the array has any blank pixels, then you can set ‘anyblank’ to 1. All the headers in ‘headers’ will also be written to this extension and ‘spack_string’ is the name of your program (which can include a version number), which will be written in the output header. -- Function: void gal_fits_atof_correct_wcs (char ‘*filename’, char ‘*hdu’, int ‘bitpix’, void ‘*array’, size_t ‘s0’, size_t ‘s1’, char ‘*wcsheader’, int ‘wcsnkeyrec’, double ‘*crpix’, char ‘*spack_string’) This is essentially the same as ‘gal_fits_array_to_file’, but through the two element ‘crpix’ array, you can change the final ‘CRPIX’ keywords that will be written in the FITS file. -- Function: void gal_fits_table_size (fitsfile ‘*fitsptr’, size_t ‘*nrows’, size_t ‘*ncols’) Get the number of rows (‘nrows’) and columns (‘ncols’) in a FITS table within the ‘fitsptr’. -- Function: int gal_fits_table_type (fitsfile ‘*fptr’) Return the type of the table: ‘ASCII_TBL’ and ‘BINARY_TBL’ for an ASCII or binary table. These two macros are defined by CFITSIO. -- Function: void gal_fits_file_or_ext_name (char ‘*inputname’, char ‘*inhdu’, int ‘othernameset’, char ‘**othername’, char ‘*ohdu’, int ‘ohduset’, char ‘*type’) This is mainly a function used in Gnuastro programs. Since a FITS image can have many extensions, usually related data are stored within one FITS file. For example an image, its masked pixels, and the sky standard deviation of the noise are various extensions of one FITS file. It would be very inconvenient if the same file name would have to be repeated in a call to a program for all images that are within one file. To easily manage things, within Gnuastro, each input variable also has an integer variable with the same name, but suffixed with ‘set’. The job of this function is to use the name of the main input image and based on the other arguments, determine what filename should be used for each type. The final argument (‘type’) is the type of input you want, for example, if you were expecting a mask image, you can give the value ‘"mask"’ as type. ‘type’ is just used to report errors. -- Function: void gal_fits_file_to_float (char ‘*inputname’, char ‘*maskname’, char ‘*inhdu’, char ‘*mhdu’, float ‘**img’, int ‘*inbitpix’, int ‘*anyblank’, size_t ‘*ins0’, size_t ‘*ins1’) Read a FITS image HDU (‘inhdu’ in ‘inputname’) as a ‘float’ type array. An optional mask image and mask hdu can also be given. Single precision floating point types are one of the most common types to store data: the observation noise is usually much larger than the extra precision (and thus volume in your computer, and slower processing) offered by double precision floating point types. With this function, so when you work internally with floating points, you can use this function to directly read a FITS image array into a floating point array. -- Function: void gal_fits_file_to_double (char ‘*inputname’, char ‘*maskname’, char ‘*inhdu’, char ‘*mhdu’, double ‘**img’, int ‘*inbitpix’, int ‘*anyblank’, size_t ‘*ins0’, size_t ‘*ins1’) Similar to ‘gal_fits_file_to_float’, but for double precision floating point type. In some contexts, the internal operations must be done in double precision floating point types, irrespective of the input type and this function can be used to directly read a file into an array of this type. -- Function: void gal_fits_file_to_long (char ‘*inputname’, char ‘*inhdu’, long ‘**img’, int ‘*inbitpix’, int ‘*anyblank’, size_t ‘*ins0’, size_t ‘*ins1’) Similar to ‘gal_fits_file_to_float’, but will read the image specified by ‘inputname’ (‘inhdu’) into a long integer type. Long integer types are commonly used to store things like segmentation maps or labeled images. -- Function: void gal_fits_prep_float_kernel (char ‘*inputname’, char ‘*inhdu’, float ‘**outkernel’, size_t ‘*ins0’, size_t ‘*ins1’) Read ‘inputname’ (‘inhdu’) will be read as a floating point array to be used as a convolution kernel. Convolution kernels are commonly necessary in astronomical image processing, but they need to have certain properties: their dimensions have to be an odd number and they must not have any blank pixels. In both cases, this function will abort with an error notice.  File: gnuastro.info, Node: Git wrappers, Next: Linked lists, Prev: FITS files, Up: Gnuastro library 10.2.5 Git wrappers (‘git.h’) ----------------------------- Git is one of the most common tools for version control and it can often be useful during development, for example see ‘COMMIT’ keyword in *note Output headers::. The functions introduced here are described in the ‘gnuastro/git.h’ header. At installation time, Gnuastro will also check for the existence of libgit2 and store the value in the ‘GAL_GNUASTRO_HAVE_LIBGIT2’, see *note Installation information::. ‘gnuastro/git.h’ includes ‘gnuastro/gnuastro.h’ internally, so won’t have to include both for this macro. -- Function: char * gal_git_describe ( ) When libgit2 is present and the program is called within a directory that is version controlled, then this function will return a string containing the commit description (similar to Gnuastro’s unofficial version number, see *note Version numbering::). If there are uncommitted changes in the running directory, it will add a ‘‘-dirty’’ prefix to the description. When there is no tagged point in the previous commit, this function will return a uniquely abbreviated commit object as fallback. This function is used for generating the value of the ‘COMMIT’ keyword in *note Output headers::. The output string is similar to the output of the following command: $ git describe --dirty --always Space for the output string is allocated within this function, so after using the value you have to ‘free’ the output string. If libgit2 is not installed or the program calling this function is not within a version controlled directory, then the output will be the ‘NULL’ pointer.  File: gnuastro.info, Node: Linked lists, Next: Mesh grid for an image, Prev: Git wrappers, Up: Gnuastro library 10.2.6 Linked lists (‘linkedlist.h’) ------------------------------------ An array is a contiguous region of memory that is very efficient and easy to use for recording and later accessing the data. One major problem with an array is that the number of elements that go into it must be known in advance. This is where linked lists can be very useful: like a metal chain, each _node_ in a linked list is an independent C structure, keeping its own data along with pointer(s) to its immediate neighbor(s). Below we have one simple linked list node structure along with an ASCII art schematic of how we can use the ‘next’ pointer to add any number of elements to the list that we want. The linked list is terminated when ‘next’ is a ‘NULL’ pointer. struct float_ll /* --------- --------- */ { /* | Value | | Value | */ float value; /* | --- | | --- | */ struct ll_node *next; /* | next-|--> | next-|--> NULL */ } /* --------- --------- */ The schematic shows another great advantage of linked lists: it is very easy to add or remove a node anywhere in the list (you just have to change one pointer in the structure above). You initially define a variable of this type with a ‘NULL’ pointer as shown below, then you use functions provided for that type of linked list to add elements to the list or pop elements from it. struct float_ll *mylist=NULL When you add an element to the list, it is conventionally added to the “top†of the list: the general list pointer will point to the newly created node, which will point to the previously created node and so on. So when you “pop†from the top of the list, you are actually retrieving the last value you put in and changing the list pointer to the next oldest node. This is thus known as a “last-in-first-out†list. This is the most convenient type of linked list (easier to implement and faster to process). Alternatively, you can add each newly created node at the end of the list. If you do that, you will get a “first-in-first-out†list. But that will force you to go through the whole list for each new element that is created (this can slow down the processing)(1). Each node in a linked list doesn’t have to have a single pointer to the next node like the example above. We can define each node with two pointers to both the next and previous neighbors, this is called a “Doubly linked listâ€. In general, lists are very powerful and simple constructs that can be very useful. But going into more detail would be out of the scope of this short introduction in this book. Wikipedia (https://en.wikipedia.org/wiki/Linked_list) has a nice and more thorough discussion of the various types of lists, so for more, please have a look at that article. In this section we will review the functions and structures that are available in Gnuastro for working on linked lists. For each linked-list node structure, we will first introduce the structure, then the functions for working on the structure. All these structures and functions are defined and declared in ‘gnuastro/linkedlist.h’. -- Structure: gal_linkedlist_fll Float linked list (‘fll’). Each node in this singly-linked list can have a single float type value. struct gal_linkedlist_fll { float v; struct gal_linkedlist_fll *next; }; -- Function: void gal_linkedlist_print_fll_array (struct gal_linkedlist_fll ‘**afll’, size_t ‘num’) Print all the values within the linked list to the output terminal. This can be used for inspecting the status of the list during development. -- Function: void gal_linkedlist_add_to_fll (struct gal_linkedlist_fll ‘**list’, float ‘value’) Allocate space for a new node in ‘list’, and put ‘value’ into it. The new node will be added to the top of the list. So after this function, the already existing nodes will be appended to the new node and ‘list’ will point to the newly created node. -- Function: void gal_linkedlist_pop_from_fll (struct gal_linkedlist_fll ‘**list’, float ‘*value’) Pop a node from the top of ‘list’ and put its values in ‘value’. This function will also free the allocated space for the popped node and after this function, ‘list’ will point to the next node. -- Function: size_t gal_linkedlist_num_in_fll (struct gal_linkedlist_fll ‘*list’) Return the number of nodes in ‘list’, the contents of ‘list’ will be untouched. -- Function: void gal_linkedlist_fll_to_array (struct gal_linkedlist_fll ‘*list’, float ‘**f’, size_t ‘*num’) Put the elements of ‘list’ into an array ‘f’ and store the number of nodes in the list in ‘num’. The array will be filled in the same order as popped elements from the list. This function will allocate space for the ‘num’ element ‘f’ array internally, so you have to free it afterwards. -- Function: void gal_linkedlist_free_fll (struct gal_linkedlist_fll ‘*list’) Free the space for all the nodes in ‘list’. Note that any values within the nodes will also be discarded. This can be used when the list is no longer relevant for you. For example, you might have already converted the list to an array for future usage with ‘gal_linkedlist_fll_to_array’. -- Function: void gal_linkedlist_free_fll_array (struct gal_linkedlist_fll ‘**afll’, size_t ‘num’) Free an array of ‘gal_linkedlist_fll’ linked lists (‘num’ elements). Each element of the array is a pointer to a linked list, so we first need to free the separate linked lists, then the array. -- Structure: gal_linkedlist_tdll Two doubles linked list (‘tdll’. Each node in this singly-linked list can have two double type values. It can be used to store an unknown number of floating point coordinates (for example RA and Dec). struct gal_linkedlist_tdll { double a; double b; struct gal_linkedlist_tdll *next; }; -- Function: void gal_linkedlist_add_to_tdll (struct gal_linkedlist_tdll ‘**list’, double ‘a’, double ‘b’) Allocate space for a new node in ‘list’, and put the values ‘a’ and ‘b’ into it. The new node will be added to the top of the list. So after this function, the already existing nodes will be appended to the new node and ‘list’ will point to the newly created node. -- Function: void gal_linkedlist_pop_from_tdll (struct gal_linkedlist_tdll ‘**list’, double ‘*a’, double ‘*b’) Pop a node from the top of ‘list’ and put its values in ‘a’ and ‘b’. This function will also free the allocated space for the popped node and after this function, ‘list’ will point to the next node. -- Function: size_t gal_linkedlist_num_int_dll (struct gal_linkedlist_tdll ‘*list’) Return the number of nodes in ‘list’. The contents of ‘list’ will be untouched. -- Function: void gal_linkedlist_tdll_to_array_inv (struct gal_linkedlist_tdll ‘*list’, double ‘**d’, size_t ‘*num’) Put the elements of ‘list’ into an array ‘d’ in inverse order and store the number of nodes in the list in ‘num’. This function will allocate space for the $2\times$‘num’ element array internally so you have to free it afterwards. The two values for each node will be stored adjacently, so the array can be seen as a 2D array with ‘num’ rows and 2 columns. -- Function: void gal_linkedlist_free_tdll (struct gal_linkedlist_tdll ‘*list’) Free the space for all the nodes in ‘list’. Note that any values within the nodes will also be discarded. This can be used when the list is no longer relevant for you. For example, you might have already converted the list to an array for future usage with ‘gal_linkedlist_tdll_to_array_inv’. -- Structure: gal_linkedlist_stll String linked list (‘stll’. Each node in this singly-linked list has a string variable. struct gal_linkedlist_stll { char *v; struct gal_linkedlist_stll *next; }; -- Function: void gal_linkedlist_add_to_stll (struct gal_linkedlist_stll ‘**list’, char ‘*value’) Allocate space for a new node in ‘list’, and store the ‘value’ pointer into it. The new node will be added to the top of the list. So after this function, the already existing nodes will be appended to the new node and ‘list’ will point to the newly created node. It is important to remember that this function will only copy the pointer in the node, it will not allocate space for the string. So the string either has to be a literal string (with a fixed address) or dynamically allocated when this linked list is to be filled and used within one function. -- Function: void gal_linkedlist_pop_from_stll (struct gal_linkedlist_stll ‘**list’, char ‘**value’) Pop a node from the top of ‘list’ and put its pointer in ‘value’. This function will also free the allocated space for the popped node and after this function, ‘list’ will point to the next node. -- Function: void gal_linkedlist_reverse_stll (struct gal_linkedlist_stll ‘**list’) Reverse the linked list. The ‘gal_linkedlist_add_to_stll’ function will make a last-in-first-out list, but commonly you will need a first-in-first-out list. This function can thus be useful after adding to the list has finished. -- Function: void gal_linkedlist_print_stll (struct gal_linkedlist_stll ‘*list’) Print all the values within the linked list to the output terminal. This can be used for inspecting the status of the list during development. -- Function: size_t gal_linkedlist_num_in_stll (struct gal_linkedlist_stll ‘*list’) Return the number of nodes in ‘list’. The contents of ‘list’ will be untouched. -- Structure: gal_linkedlist_sll ‘size_t’ linked list (‘sll’. Each node in this singly-linked list contains a ‘size_t’ value. The ‘size_t’ type is commonly used for “size†related values: it is an un-signed type (negative values are not defined for it), therefore it is ideal for dealing with things like pixel indexes in an image (which can not be negative and can be very large). struct gal_linkedlist_sll { size_t v; struct gal_linkedlist_sll *next; }; -- Function: void gal_linkedlist_add_to_sll (struct gal_linkedlist_sll ‘**list’, size_t ‘value’) Allocate space for a new node in ‘list’, and store ‘value’ into it. The new node will be added to the top of the list. So after this function, the already existing nodes will be appended to the new node and ‘list’ will point to the newly created node. -- Function: void gal_linkedlist_pop_from_sll (struct gal_linkedlist_sll ‘**list’, size_t ‘*value’) Pop a node from the top of ‘list’ and put its value in ‘value’. This function will also free the allocated space for the popped node and after this function, ‘list’ will point to the next node. -- Function: size_t gal_linkedlist_num_in_sll (struct gal_linkedlist_sll ‘*list’) Return the number of nodes in ‘list’. The contents of ‘list’ will be untouched. -- Function: void gal_linkedlist_print_sll (struct gal_linkedlist_sll ‘*list’) Print all the values within the linked list to the output terminal. This can be used for inspecting the status of the list during development. -- Function: void gal_linkedlist_sll_to_array (struct gal_linkedlist_sll ‘*list’, size_t ‘**s’, size_t ‘*num’, int ‘inverse’) Put the elements of ‘list’ into an array ‘s’ and store the number of nodes in the list in ‘num’. This function will allocate space for the ‘num’ element array internally so you have to free it afterwards. If the value in ‘inverse’ is ‘1’, then the first popped value in the list will be the last element in the array, otherwise, the array will be filled in the same order that the elements were popped. -- Function: void gal_linkedlist_free_sll (struct gal_linkedlist_sll ‘*list’) Free the space for all the nodes in ‘list’. Note that any values within the nodes will also be discarded. This can be used when the list is no longer relevant for you. For example, you might have already converted the list to an array for future usage with ‘gal_linkedlist_sll_to_array’. -- Structure: gal_linkedlist_osll Ordered ‘size_t’ linked list (‘osll’. Each node in this singly-linked list contains a ‘size_t’ value and a floating point value. The floating point value is used as a reference to add new nodes in a sorted manner. At any moment, the first popped node in this list will have the smallest ‘tosort’ value, and subsequent nodes will have larger to values. struct gal_linkedlist_osll { size_t v; float s; struct gal_linkedlist_osll *next; }; -- Function: void gal_linkedlist_add_to_osll (struct gal_linkedlist_osll ‘**list’, size_t ‘value’, float ‘tosort’) Allocate space for a new node in ‘list’, and store ‘value’ into it. The new node will be added to the list based on the ‘tosort’ value. -- Function: void gal_linkedlist_pop_from_osll (struct gal_linkedlist_osll ‘**list’, size_t ‘*value’, float ‘*sortvalue’) Pop a node from the top of ‘list’, put its value in ‘value’ and its sort value in ‘sortvalue’. This function will also free the allocated space for the popped node and after this function, ‘list’ will point to the next node (which has a larger ‘tosort’ element). -- Function: void gal_linkedlist_osll_into_sll (struct gal_linkedlist_osll ‘*in’, struct gal_linkedlist_sll ‘**out’) Convert the orderd ‘size_t’ linked list into an ordinary ‘size_t’ linked list (no longer sorted). This can be useful when all the elements have been added and you just need to pop-out elements. -- Structure: gal_linkedlist_tosll Two-way, ordered ‘size_t’ linked list (‘tosll’. Each node in this Doubly-linked list contains a ‘size_t’ value and a floating point value. The floating point value is used as a reference to add new nodes in a sorted manner. In the functions here, this linked list can be pointed to by two pointers (largest and smallest) with the following format: largest pointer | NULL <-- (v0,s0) <--> (v1,s1) <--> ... (vn,sn) --> NULL | smallest pointer At any moment, the two pointers will point the nodes containing the “largest†and “smallest†values and the rest of the nodes will be sorted. This is useful when an unknown number of nodes are being added continuously and during the operations it is important to have the nodes in a sorted format. struct gal_linkedlist_tosll { size_t v; float s; struct gal_linkedlist_tosll *prev; struct gal_linkedlist_tosll *next; }; -- Function: void gal_linkedlist_print_tosll (struct gal_linkedlist_tosll ‘*largest’, struct gal_linkedlist_tosll ‘*smallest’) Print all the values within the linked list to the output terminal. This can be used for inspecting the status of the list during development. -- Function: void gal_linkedlist_add_to_tosll_end (struct gal_linkedlist_tosll ‘**largest’, struct gal_linkedlist_tosll ‘**smallest’, size_t ‘value’, float ‘tosort’) Allocate space for a new node in ‘list’, and store ‘value’ into it. The new node will be added to the list based on the ‘s’ value as described in the description of ‘gal_linkedlist_tosll’. If this is the first node to be added to the list, both the ‘largest’ and ‘smallest’ pointers can be ‘NULL’. -- Function: void gal_linkedlist_pop_from_tosll_start (struct gal_linkedlist_tosll ‘**lartest’, struct gal_linkedlist_tosll ‘**smallest’, size_t ‘*value’, float ‘*tosort’) Pop the node with the smallest ‘s’ of ‘list’, then put its value in ‘value’ and its sort value in ‘sortvalue’. This function will also free the allocated space for the popped node and after this function, ‘largest’ and ‘smallest’ will be modified respectively. Note that even though only the smallest pointer will be popped, when there was only one node in the list, the ‘largest’ pointer also has to change, so we need both. -- Function: void gal_linkedlist_smallest_tosll (struct gal_linkedlist_tosll ‘*largest’, struct gal_linkedlist_tosll ‘**smallest’) Given the ‘largest’ pointer, set ‘smallest’ as described in ‘gal_linkedlist_tosll’. -- Function: void gal_linkedlist_tosll_into_sll (struct gal_linkedlist_tosll ‘*in’, struct gal_linkedlist_sll ‘**out’) Convert the two-way orderd ‘size_t’ linked list into an ordinary ‘size_t’ linked list (no longer sorted). This can be useful when all the elements have been added and you just need to pop-out elements. -- Function: void gal_linkedlist_tosll_free (struct gal_linkedlist_tosll ‘*largest’) Free the space for all the nodes in ‘largest’. Note that any values within the nodes will also be discarded. ---------- Footnotes ---------- (1) A better way to get a first-in-first-out is to first keep the data as last-in-first-out until they are all read. Afterwards, pop each node and immediately add it to the new list: practically reversing the last-in-first-out list to a first-in-first-out one.  File: gnuastro.info, Node: Mesh grid for an image, Next: Polygons, Prev: Linked lists, Up: Gnuastro library 10.2.7 Mesh grid for an image (‘mesh.h’) ---------------------------------------- The basic concepts behind the mesh and channel grids in Gnuastro were explained in *note Tiling an image::. Besides the improved measurement purposes introduced there, tiling an image can also greatly speed up some processing operations over the image, since each mesh can be given to a different thread and so the CPU can be working on multiple regions of the image simultaneously. The mesh structure and functions introduced here are declared in ‘gnuastro/mesh.h’ and allow you to also use operate on an image mesh. Please note that as discussed in *note Gnuastro library::, most library functions will significantly evolve with future releases. The mesh structure and functions introduced here are high on this list: until now they were only internally used and so not much attention had been paid to their usability outside Gnuastro. Gnuastro’s ‘lib/mesh.c’ contains the full function definitions and is heavily commented, please also consult that file if the explanations here are not clear enough. However, the basic idea behind this structure, and the functions to manipulate data over it, is a powerful tool that can be generically used in many contexts. So please use the structure and functions here very critically and share your criticisms, thoughts and ideas on them. Hopefully in future releases the structure and functions were will evolve to become an easy to use and generically applicable mesh grid system. -- Structure: gal_mesh_params This structure keeps all the necessary parameters for a particular mesh and channel grid over an image. This structure only keeps the information about the mesh and channel grid structure. It doesn’t keep a copy of the different parts of the image. So when working on several images of the same size, you can use the same mesh structure. Its individual elements are too many to fully list here, if you are interested please look into the installed ‘gnuastro/mesh.h’ header. One important component of the structure which is commonly used in the functions is the ‘garray’, where each mesh has a unique ‘gid’. ‘garray’ stands for grid-array. It is used for operations on the mesh grid, where one value is to be assigned for each mesh. It has one element for each mesh in the image. However, due to the (possible) existence of channels (see *note Tiling an image::), each channel needs its own contiguous part (group of meshes) in the full ‘garray’. Each channel has ‘gs0*gs1’ (dimensions of meshes in each channel) elements. There are ‘nch’ parts (or channels) in total. In short, the meshs in each channel have to be contiguous to facilitate the neighbor analysis in interpolation and other channel specific jobs. So, the over-all structure can be viewed as a 3D array. The operations on the meshs might need more than one output, for example the mean and the standard deviation. So we have two ‘garray’s and two ‘nearest’ arrays (for interpolation). -- Function: size_t gal_mesh_ch_based_id_from_gid (struct gal_mesh_params ‘*mp’, size_t ‘gid’) As discussed in the description of ‘gal_mesh_params’, there are two internal ways to refer to a mesh (with an ID): • By default, the mesh IDs are set based on their position within the channels (so the meshs in each channel are contiguous). We call this the channel-based mesh ID. The ‘cgarray1’ and ‘cgarray2’ in ‘gal_mesh_params’ store the mesh values based on this ID. All the basic mesh properties, like their types and height and widths are stored based on this ID. • If the user asks for a full image interpolation or smoothing, then two new arrays are created called ‘fgarray1’ and ‘fgarray2’. These arrays keep the mesh values as they appear on the image, irrespective of which channel they belong to. We call this the image-based ID. The image based ID is contiguous over the image. The ‘garray1’ and ‘garray2’ pointers can point to either the ‘cgarrays’ or the ‘fgarrays’. Ideally, the user should not worry about what garray is pointing to. The caller knows the type of IDs they are using, but they don’t know what to put into ‘garray’. We call the ID that should be put into garray the channel-based ID. It can be either of the two kinds above. So we have the following two functions ‘gal_mesh_ch_based_id_from_gid’ and ‘gal_mesh_gid_from_ch_based_id’ for changing between these IDs. The former (this function) is used when you are going over the elements in garray (and you are completely ignorant to which one of cgarrays or fgarrays garray points to) and you need the channel based IDs to get basic mesh information like the mesh type and size. -- Function: size_t gal_mesh_gid_from_ch_based_id (struct gal_mesh_params ‘*mp’, size_t ‘chbasedid’) See the explanations in ‘gal_mesh_ch_based_id_from_gid’ first. This function is used when you are going over the meshs through the channel-based IDs, but you need to know what ID to use for ‘garray’. -- Function: size_t gal_mesh_img_xy_to_mesh_id (struct gal_mesh_params ‘*mp’, size_t ‘x’, size_t ‘y’) You have a pixel’s position as ‘x’ and ‘y’ in the final image (in C-based dimensions) and want to know the id to be used in the ‘garray’s to get a value for this pixel in the mesh-grid. This function will return that ID. As an example, you can get the mesh value at a specific position in the image with: mp->garray[ gal_mesh_img_xy_to_mesh_id(mp, x, y) ]; -- Function: void gal_mesh_check_mesh_id (struct gal_mesh_params ‘*mp’, long ‘**out’) Save the meshid of each pixel into an array the size of the original image. All the pixels over the mesh will get the value of the mesh ID. The output array ‘out’ can then be written to a FITS file for viewing. This is mainly used for checking/debugging purposes, hence the ‘check’ in the name. -- Function: void gal_mesh_check_garray (struct gal_mesh_params ‘*mp’, float ‘**out1’, float ‘**out2’) Save the values in the ‘garray’s of the input ‘mp’ structure into two arrays the size of the input image. All the pixels over each mesh will get the value corresponding to that mesh in the ‘garray’s. The output arrays can then be written to a FITS file for viewing. This is mainly used for checking/debugging purposes, hence the ‘check’ in the name. ‘out2’ will only be set if there are two ‘garray’s. -- Function: void gal_mesh_value_file (struct gal_mesh_params ‘*mp’, char ‘*filename’, char ‘*extname1’, char ‘*extname2’, struct wcsprm ‘*wcs’, char ‘*spack_string’) Save the mesh grid values into the ‘filename’ FITS file with ‘extname1’ and ‘extname2’ extension names (for the two possible ‘garrays’), a WCS structure may also optionally be given and ‘spack_string’ is the name of your program to be written in the header. The output FITS file will have one pixel for each mesh, so its dimensions will be significantly smaller than the input image. If you want the mesh values in the same dimension as the input image, use ‘gal_mesh_check_garray’. -- Function: void gal_mesh_full_garray (struct gal_mesh_params ‘*mp’, int ‘reverse’) As described in ‘gal_mesh_ch_based_id_from_gid’, the there can be two arrays that keep a value for each mesh in ‘gal_mesh_params’: ‘cgarray’ and ‘fgarray’. When ‘reverse==0’, then this function will fill in the ‘fgarray’s using the ‘cgarray’s and vice-versa when ‘reverse==1’. -- Function: void gal_mesh_make_mesh (struct gal_mesh_params ‘*mp’) Make the mesh structure using the basic information that must already be present within it. The complete list of necessary parameters are as follows, but note that some might not be necessary for your desired functionality. ‘s0’, ‘s1’, ‘ks0’, ‘ks1’, ‘nch1’, ‘nch2’, ‘kernel’, ‘img’, ‘params’, ‘minmodeq’, ‘mirrordist’, ‘fullsmooth’, ‘numnearest’, ‘smoothwidth’, ‘lastmeshfrac’, ‘meshbasedcheck’, ‘interponlyblank’, ‘fullinterpolation’, ‘numthreads’. See the installed ‘gnuastro/mesh.h’ for a comment on each parameter within the ‘gal_mesh_params’ structure. -- Function: void gal_mesh_free_mesh (struct gal_mesh_params ‘*mp’) Free all the allocated spaces within the ‘gal_mesh_params’ structure. -- Function: void gal_mesh_operate_on_mesh (struct gal_mesh_params ‘*mp’, void ‘*(*meshfunc)(void *)’, size_t ‘oneforallsize’, int ‘makegarray2’, int ‘initialize’) Run the ‘meshfunc’ function on each mesh in parallel. As the declaration above shows, ‘meshfunc’ should only take one ‘void *’ input and return one ‘void *’ output. This function will setup a pthread environment and make ‘mp->numthreads’ (a number!) calls ‘meshfunc’ which will work on each mesh. ‘gal_mesh_operate_on_mesh’ will return when all the threads have finished their work. If ‘meshfunc’ needs to store more than one value for each mesh, then set ‘makegarray2=1’. When ‘initialize==1’, the ‘garray’(s) will be initialized to NaN. This function is commonly used within Gnuastro (mainly in NoiseChisel, see *note NoiseChisel::), so search for its applications in the programs for some real-world examples. You can do this with the following command in the top Gnuastro source directory (after unpacking the tarball): grep -r gal_mesh_operate_on_mesh ./bin/* -- Function: void gal_mesh_interpolate (struct gal_mesh_params ‘*mp’, char ‘*errstart’) Interpolate the mesh values (‘garray’s). After you have run a function on all the meshes with ‘gal_mesh_operate_on_mesh’, some meshes might not get any values. This function will fill the meshes that didn’t get any values (have a value of NaN) using the meshes that received a value. The interpolation is done based on the nearest neighbors, specified within the ‘gal_mesh_params’ structure. -- Function: void gal_mesh_smooth (struct gal_mesh_params ‘*mp’) Smooth the mesh values arrays based on the parameters in ‘gal_mesh_params’. -- Function: void gal_mesh_spatial_convolve_on_mesh (struct gal_mesh_params ‘*mp’, float ‘**conv’) Do spatial convolution (see *note Spatial domain convolution::) on each channel of the mesh grid independently, therefore two adjacent pixels within the image that are not in the same channel will not affect each other during the convolution. -- Function: void gal_mesh_change_to_full_convolution (struct gal_mesh_params ‘*mp’, float ‘*conv’) After running ‘gal_mesh_spatial_convolve_on_mesh’, it might become necessary to change the convolution into a full image convolution. This function will do the convolution process only on the regions near the channel borders that need to be changed, the rest of the pixels will not be changed by this function.  File: gnuastro.info, Node: Polygons, Next: Qsort functions, Prev: Mesh grid for an image, Up: Gnuastro library 10.2.8 Polygons (‘polygon.h’) ----------------------------- Polygons are commonly necessary in image processing. In Gnuastro, they are used in ImageCrop (see *note ImageCrop::) for cutting out non-rectangular regions of a image. ImageWarp (see *note ImageWarp::) uses them to warp the images into a new pixel grid. The polygon related Gnuastro library macros and functions are introduced here. In all the functions here the vertices (and points) are defined as an array. So a polygon with 4 vertices will be identified with an array of 8 elements with the first two elements keeping the 2D coordinates of the first vertice and so on. -- Macro: GAL_POLYGON_MAX_CORNERS The largest number of vertices a polygon can have in this library. -- Macro: GAL_POLYGON_ROUND_ERR We have to consider floating point round-off errors when dealing with polygons. For example we will take ‘A’ as the maximum of ‘A’ and ‘B’ when ‘A>B-GAL_POLYGON_ROUND_ERR’. -- Function: void gal_polygon_ordered_corners (double ‘*in’, size_t ‘n’, size_t ‘*ordinds’) We have a simple polygon (that can result from projection, so its edges don’t collide or it doesn’t have holes) and we want to order its corners in an anticlockwise fashion. This is necessary for clipping it and finding its area later. The input vertices can have practically any order. The input (‘in’) is an array containing the coordinates (two values) of each vertice. ‘n’ is the number of corners. So ‘in’ should have ‘2*n’ elements. The output (‘ordinds’) is an array with ‘n’ elements specifying the indexs in order. This array must have been allocated before calling this function. The indexes are output for more generic usage, for example in a homographic transform (necessary in warping an image, see *note Warping basics::), the necessary order of vertices is the same for all the pixels. In other words, only the positions of the vertices change, not the way they need to be ordered. Therefore, this function would only be necessary once. As a summary, the input is unchanged, only ‘n’ values will be put in the ‘ordinds’ array. Such that calling the input coordinates in the following fashion will give an anti-clockwise order when there are 4 vertices: 1st vertice: in[ordinds[0]*2], in[ordinds[0]*2+1] 2nd vertice: in[ordinds[1]*2], in[ordinds[1]*2+1] 3rd vertice: in[ordinds[2]*2], in[ordinds[2]*2+1] 4th vertice: in[ordinds[3]*2], in[ordinds[3]*2+1] The implementation of this is very similar to the Graham scan in finding the Convex Hull. However, in projection we will never have a concave polygon (the left condition below, where this algorithm will get to E before D), we will always have a convex polygon (right case) or E won’t exist! Concave Polygon Convex Polygon D --------C D------------- C \ | E / | \E | \ | / | \ | A--------B A ----------B This is because we are always going to be calculating the area of the overlap between a quadrilateral and the pixel grid or the quadrilaterral its self. The ‘GAL_POLYGON_MAX_CORNERS’ macro is defined so there will be no need to allocate these temporary arrays separately. Since we are dealing with pixels, the polygon can’t really have too many vertices. -- Function: double gal_polygon_area (double ‘*v’, size_t ‘n’) Find the area of a polygon with vertices defined in ‘v’. ‘v’ points to an array of doubles which keep the positions of the vertices such that ‘v[0]’ and ‘v[1]’ are the positions of the first vertice to be considered. -- Function: int gal_polygon_pin (double ‘*v’, double ‘*p’, size_t ‘n’) Return ‘1’ if the point ‘p’ is within the polygon whose vertices are defined by ‘v’ and ‘0’ otherwise. Note that the vertices of the polygon have to be sorted in an anti-clock-wise manner. -- Function: int gal_polygon_ppropin (double ‘*v’, double ‘*p’, size_t ‘n’) Similar to ‘gal_polygon_pin’, except that if the point ‘p’ is on one of the edges of a polygon, this will return ‘0’. -- Function: void gal_polygon_clip (double ‘*s’, size_t ‘n’, double ‘*c’, size_t ‘m’, double ‘*o’, size_t ‘*numcrn’) Clip (find the overlap of) two polygons. This function uses the Sutherland-Hodgman (https://en.wikipedia.org/wiki/Sutherland%E2%80%93Hodgman_algorithm) polygon clipping algorithm. Note that the vertices of both polygons have to be sorted in an anti-clock-wise manner.  File: gnuastro.info, Node: Qsort functions, Next: Spatial convolution, Prev: Polygons, Up: Gnuastro library 10.2.9 Qsort functions (‘qsort.h’) ---------------------------------- The C programming language comes with the ‘qsort’ (Quick sort) function. By allowing you to define the sorting based on the data, ‘qsort’ is a generic function which allows you to sort any kind of data structure. The functions here are all meant to be passed onto ‘qsort’ for sorting the respective types of data in the respective manner. Because of this all these functions have the same two argument types. -- Global variable: gal_qsort_index_arr Pointer to a floating point array (‘float *’) to use as a reference in ‘gal_qsort_index_float_decreasing’, see the explanation there for more. -- Function: int gal_qsort_int_decreasing (const void ‘*a’, const void ‘*b’) When passed to ‘qsort’, this function will sort an integer array in decreasing order. -- Function: int gal_qsort_int_increasing (const void ‘*a’, const void ‘*b’) When passed to ‘qsort’, this function will sort an integer array in increasing order. -- Function: int gal_qsort_float_decreasing (const void ‘*a’, const void ‘*b’) When passed to ‘qsort’, this function will sort a single precision floating point array in decreasing order. -- Function: int gal_qsort_float_increasing (const void ‘*a’, const void ‘*b’) When passed to ‘qsort’, this function will sort a single precision floating point array in increasing order. -- Function: int gal_qsort_double_decreasing (const void ‘*a’, const void ‘*b’) When passed to ‘qsort’, this function will sort a double precision floating point array in decreasing order. -- Function: int gal_qsort_double_increasing (const void ‘*a’, const void ‘*b’) When passed to ‘qsort’, this function will sort a double precision floating point array in increasing order. -- Function: int gal_qsort_index_float_decreasing (const void ‘*a’, const void ‘*b’) When passed to ‘qsort’, this function will sort a ‘size_t’ array based on decreasing values in the ‘gal_qsort_index_arr’ single precision floating point array. The floating point array will not be changed, it is only read. For example, if we have the following source code: #include #include /* qsort is defined in stdlib.h. */ #include int main (void) { size_t s[4]={0, 1, 2, 3}; float f[4]={1.3,0.2,1.8,0.1}; gal_qsort_index_arr=f; qsort(s, 4, sizeof(size_t), gal_qsort_index_float_decreasing); printf("%zu, %zu, %zu, %zu\n", s[0], s[1], s[2], s[3]); return EXIT_SUCCESS; } The output will be: ‘2, 0, 1, 3’.  File: gnuastro.info, Node: Spatial convolution, Next: Statistical operations, Prev: Qsort functions, Up: Gnuastro library 10.2.10 Spatial convolution (‘spatialconvolve.h’) ------------------------------------------------- Convolution is a common operation in data processing and is fully explained in *note Spatial domain convolution:: as part of *note Convolve::. We will therefore not explain the details, or its purpose here. The main high-level function here is ‘gal_spatialconvolve_convolve’ which will do spatial convolution on multiple threads. The structure and functions introduced here are declared in ‘gnuastro/spatialconvolve.h’. In the first release of the Gnuastro libraries, this is the most high-level library since it was needed by multiple programs. In future releases this library will most probably merge with the frequency domain convolution functions to allow programmers to choose from the type of convolution they want. The main -- Structure: gal_spatialconvolve_params This structure keeps all the basic convolution information so subsequent calls can be simpler. Please see the header for the details of its elements, complemented with comments. -- Function: void gal_spatialconvolve_pparams (float ‘*input’, size_t ‘is0’, size_t ‘is1’, float ‘*kernel’, size_t ‘ks0’, size_t ‘ks1’, size_t ‘nt’, int ‘edgecorrection’, float ‘*out’, size_t ‘*indexs’, struct gal_spatialconvolve_params ‘*scp’) Initialize ‘gal_spatialconvolve_params’ with the given arguments. -- Function: void * gal_spatialconvolve_thread (void ‘*inparam’) This function should be passed onto ‘pthread_create’ to create a new thread for convolution on a region of the image. -- Function: void gal_spatialconvolve_convolve (float ‘*input’, size_t ‘is0’, size_t ‘is1’, float ‘*kernel’, size_t ‘ks0’, size_t ‘ks1’, size_t ‘numthreads’, int ‘edgecorrection’, float ‘**out’) Convolve ‘input’ (with ‘is0*is1’ pixels) with the ‘kernel’ (with ‘ks0*ks1’) on ‘numthreads’ CPU threads. If you want edge-correction (see *note Edges in the spatial domain::), then set ‘edgecorrection’ to ‘1’, otherwise set it to ‘0’. Memory will be allocated for the output and the convolved image will be stored in ‘out’.  File: gnuastro.info, Node: Statistical operations, Next: Multithreaded programming, Prev: Spatial convolution, Up: Gnuastro library 10.2.11 Statistical operations (‘statistics.h’) ----------------------------------------------- This header includes a large variety of very basic statistical operators for various data types. Please note that we expect to greatly simplify the functions here for easier and more general usage in future releases. Ideally, they should be completely removed and the GNU Scientific Library’s functions should be used. Since these functions are used in various parts of Gnuastro for multiple purposes, in this first library release (Gnuastro 0.2), there might be parallels, or non-homogeneous arguments. Such situations arise here because of the history of Gnuastro: the libraries grew out of the programs, so it will take a little while to correct. -- Structure: GAL_STATISTICS_MAX_SIG_CLIP_CONVERGE The maximum number of times to try for $\sigma$-clipping (see *note Sigma clipping::). -- Function: void gal_statistics_long_non_blank_min (long ‘*in’, size_t ‘size’, long ‘*min’, long ‘blank’) Find the the minimum (non-blank) value in the ‘in’ array (with ‘size’ elements). The long type doesn’t have a NaN value like the float types, see *note Blank pixels::. So as blank pixels, a value in the range of acceptable values (‘blank’ must be given so it is explicitly ignored. You can use ‘GAL_FITS_LONG_BLANK’ in ‘gnuastro/fits.h’. -- Function: void gal_statistics_long_non_blank_max (long ‘*in’, size_t ‘size’, long ‘*max’, long ‘blank’) Similar to ‘gal_statistics_long_non_blank_min’, but find the maximum. -- Function: void gal_statistics_float_min (float ‘*in’, size_t ‘size’, float ‘*min’) Find the minimum value in the single precision floating point ‘in’ array (with ‘size’ elements) and store the value in ‘min’. Note that for all floating point types, any blank (NaN) value will be automatically ignored in this function. -- Function: void gal_statistics_float_max (float ‘*in’, size_t ‘size’, float ‘*max’) Similar to ‘gal_statistics_float_min’ but find the maximum. -- Function: void gal_statistics_double_min (double ‘*in’, size_t ‘size’, double ‘*min’) Similar to ‘gal_statistics_float_min’ but for double precision floating point types. -- Function: double gal_statistics_double_min_return (double ‘*in’, size_t ‘size’) Similar to ‘gal_statistics_double_min’ but minimum will be returned, not put in a pointer. -- Function: void gal_statistics_double_max (double ‘*in’, size_t ‘size’, double ‘*max’) Similar to ‘gal_statistics_double_min’, but find maximum value. -- Function: double gal_statistics_double_max_return (double ‘*in’, size_t ‘size’) Similar to ‘gal_statistics_double_max_return’, but return maximum. -- Function: void gal_statistics_float_max_masked (float ‘*in’, unsigned char ‘*mask’, size_t ‘size’, float ‘*max’) Only find maximum where ‘mask’ has a value of ‘0’. -- Function: void gal_statistics_float_second_max (float ‘*in’, size_t ‘size’, float ‘*secondmax’) Find the second largest value in the array. -- Function: void gal_statistics_float_second_min (float ‘*in’, size_t ‘size’, float ‘*secondmin’) Find the second smallest value in the array. -- Function: void gal_statistics_f_min_max (float ‘*in’, size_t ‘size’, float ‘*min’, float ‘*max’) Find the minimum and maximum simultaneously for single precision floating point types. -- Function: void gal_statistics_d_min_max (double ‘*in’, size_t ‘size’, double ‘*min’, double ‘*max’) Similar to ‘gal_statistics_f_min_max’, but for double precision floating point types. -- Function: void gal_statistics_f_max_with_index (float ‘*in’, size_t ‘size’, float ‘*max’, size_t ‘*index’) Find the maximum value in the array along with its index for a single precision floating point array. -- Function: void gal_statistics_d_max_with_index (double ‘*in’, size_t ‘size’, double ‘*max’, size_t ‘*index’) Similar to ‘gal_statistics_f_max_with_index’, but for a double precision floating point array. -- Function: void gal_statistics_d_min_with_index (double ‘*in’, size_t ‘size’, double ‘*min’, size_t ‘*index’) -- Function: void gal_statistics_f_min_with_index (float ‘*in’, size_t ‘size’, float ‘*min’, size_t ‘*index’) -- Function: float gal_statistics_float_sum (float ‘*in’, size_t ‘size’) Return the sum of the single precision floating point arrays. Note that NaN values will be ignored. -- Function: float gal_statistics_float_sum_num (float ‘*in’, size_t ‘*size’) Return the sum of elements in the floating point array along with the number of used (non-Nan) elements. -- Function: float gal_statistics_float_sum_squared (float ‘*in’, size_t ‘size’) Return the sum of squares of non-NaN elements in the array. -- Function: float gal_statistics_float_sum_mask (float ‘*in’, unsigned char ‘*mask’, size_t ‘size’, size_t ‘*nsize’) Given a mask (‘mask’), return the sum of elements with a ‘mask’ value of ‘0’ (masked pixels are considered to have a non-zero value) and put the number of used elements in ‘nsize’. -- Function: float gal_statistics_float_sum_mask_l (float ‘*in’, long ‘*mask’, size_t ‘size’, size_t ‘*nsize’) Similar to ‘gal_statistics_float_sum_mask’, but when the mask is a long type. -- Function: float gal_statistics_float_sum_squared_mask (float ‘*in’, unsigned char ‘*mask’, size_t ‘size’, size_t ‘*nsize’) Return the sum of the squared elements in ‘in’ that are not masked (corresponding element in ‘mask’ is ‘0’. -- Function: float gal_statistics_float_sum_squared_mask_l (float ‘*in’, long ‘*mask’, size_t ‘size’, size_t ‘*nsize’) Similar to ‘gal_statistics_float_sum_squared_mask’ but when the mask is a long type. -- Function: float gal_statistics_float_average (float ‘*in’, size_t ‘size’) Return the average of the single precision floating point array ‘in’ with ‘size’ elements. -- Function: double gal_statistics_double_average (double ‘*in’, size_t ‘size’) Return the average of the double precision floating point array ‘in’ with ‘size’ elements. -- Function: void gal_statistics_f_ave (float ‘*in’, size_t ‘size’, float ‘*ave’, unsigned char ‘*mask’) Return the average of the single precision floating point array ‘in’ with ‘size’ elements, do not use those elements where ‘mask’ is non-zero. -- Function: void gal_statistics_f_ave_l (float ‘*in’, size_t ‘size’, float ‘*ave’, long ‘*mask’) Similar to ‘gal_statistics_f_ave’, but when the mask is of type long. -- Function: void gal_statistics_f_ave_std (float ‘*in’, size_t ‘size’, float ‘*ave’, float ‘*std’, unsigned char ‘*mask’) Find the average and standard deviation of the ‘in’ array for pixels where ‘mask’ has value of ‘0’. -- Function: void gal_statistics_f_ave_std_l (float ‘*in’, size_t ‘size’, float ‘*ave’, float ‘*std’, long ‘*mask’) Similar to ‘gal_statistics_f_ave_std’, but when the mask has a type of long. -- Function: float gal_statistics_median (float ‘*array’, size_t ‘insize’) Return the median value of a single precision floating point array ‘array’ (which has ‘insize’ elements). -- Function: double gal_statistics_median_double_in_place (double ‘*array’, size_t ‘insize’) Return the median value of a double precision floating point array ‘array’ (which has ‘insize’ elements). After this function, the elements of ‘array’ are also sorted. -- Function: void gal_statistics_set_bins (float ‘*sorted’, size_t ‘size’, size_t ‘numbins’, float ‘min’, float ‘max’, float ‘onebinvalue’, float ‘quant’, float ‘**obins’) Given the input ‘sorted’ array with ‘size’ elements, a given number of ‘numbins’, an optional ‘min’ and ‘max’, find the the bin starting points and keep them in ‘obins’. ‘obins’ has two columns, and this function only fills the first column. The second will be filled by the histogram or cumulative distribution plots. If ‘onebinvalue’ is NaN, then the bins above will be reported. However, if it is not NaN, all the bins will be shifted such that the lower value of one of the bins will be placed on this value of this variable (if it is in the range of the data). When ‘min==max’, the actual data range will be used. When ‘quant’ is not zero (let’s say it has the value $q$, for quantile) and ‘min==max’ then the automatic range finder will use the values at the quantiles $q$ and $1-q$. -- Function: void gal_statistics_histogram (float ‘*sorted’, size_t ‘size’, float ‘*bins’, size_t ‘numbins’, int ‘normhist’, int ‘maxhistone’) Build the histogram of the data (‘sorted’, with ‘size’ elements) in the ‘bins’ array which also contains the starting bin values and has ‘numbins’ rows. See ‘gal_statistics_set_bins’. When ‘normhist’ is non-zero, the histogram will be normalized so the sum of all the bin values is unity. When ‘maxhistone’ is non-zero, the histogram is scaled such that the bin with the largest value gets a value of 1. -- Function: void gal_statistics_cumulative_fp (float ‘*sorted’, size_t ‘size’, float ‘*bins’, size_t ‘numbins’, int ‘normcfp’) Build the cumulative frequency plot of the data (‘sorted’, with ‘size’ elements) in the ‘bins’ array which also contains the starting bin values and has ‘numbins’ rows. See ‘gal_statistics_set_bins’. When ‘normcfp’ is non-zero, the cumulative frequency plot will be normalized so the last bin has a value of 1. -- Function: void gal_statistics_save_hist (float ‘*sorted’, size_t ‘size’, size_t ‘numbins’, char ‘*filename’, char ‘*comment’) Create a histogram of the data in ‘sorted’ (and ‘size’ elements) with ‘numbins’ and save it into an ASCII text file named ‘filename’ with a possible set of comments (pointed to by ‘comment’ before he table. -- Function: size_t gal_statistics_index_from_quantile (size_t ‘size’, float ‘quant’) Given the number of elements (‘size’), return the index corresponding to the quantile ‘quant’. -- Function: int gal_statistics_sigma_clip_converge (float ‘*array’, int ‘o1_n0’, size_t ‘num_elem’, float ‘sigma_multiple’, float ‘accuracy’, float ‘*outave’, float ‘*outmed’, float ‘*outstd’, int ‘print’) Calculate the $\sigma$-clipped (by convergence) average, median and standard deviation on the array ‘array’ with ‘num_elem’ elements (see *note Sigma clipping::). If ‘o1_n0==1’, then it is assumed that the input array is sorted. ‘sigma_multiple’ is the multiple of $\sigma$ used in the $\sigma$-clipping. If the $\sigma$-clipping did converge, then this function will return ‘0’, otherwise, it will return ‘1’. If ‘print’ is non-zero, then the average, median and standard deviation of each step are printed. -- Function: int gal_statistics_sigma_clip_certain_num (float ‘*array’, int ‘o1_n0’, size_t ‘num_elem’, float ‘sigma_multiple’, size_t ‘numtimes’, float ‘*outave’, float ‘*outmed’, float ‘*outstd’, int ‘print’) Calculate the $\sigma$-clipped (with a fixed number of times) average, median and standard deviation on the array ‘array’ with ‘num_elem’ elements (see *note Sigma clipping::). If ‘o1_n0==1’, then it is assumed that the input array is sorted. ‘sigma_multiple’ is the multiple of $\sigma$ and ‘numtimes’ is the number of times $\sigma$-clipping is done. If the $\sigma$-clipping was normally done, then this function will return ‘0’, otherwise, it will return ‘1’. If ‘print’ is non-zero, then the average, median and standard deviation of each step are printed. -- Function: void gal_statistics_remove_outliers_flat_cdf (float ‘*sorted’, size_t ‘*outsize’) Remove the outliers in a distribution based on the slope of the cumulative frequency plot (when it becomes too flat). Before this function, ‘outssize’ will point to the number of elements in ‘sorted’, after this function, it will be the number of elements that are not outliers. -- Macro: GAL_STATISTICS_MODE_LOW_QUANTILE The lower quantile used in calculating the mode. -- Macro: GAL_STATISTICS_MODE_HIGH_QUANTILE The lower quantile used in calculating the mode. -- Macro: GAL_STATISTICS_MODE_SYM_GOOD The acceptable value for the mode calculation symmetry. -- Macro: GAL_STATISTICS_MODE_LOW_QUANT_GOOD The lowest quantile that an acceptable mode can have. -- Macro: GAL_STATISTICS_MODE_SYMMETRICITY_LOW_QUANT Lower quantile for calculating the symmetricity. -- Structure: gal_statistics_mode_params The input parameters for the mode functions, this is mainly an internal structure and will become hidden in future releases. -- Function: void gal_statistics_mode_mirror_plots (float ‘*sorted’, size_t ‘size’, size_t ‘mirrorindex’, float ‘min’, float ‘max’, size_t ‘numbins’, char ‘*histsname’, char ‘*cfpsname’, float ‘mirrorplotdist’) Create a mirror plot based on the index given by ‘mirrorindex’. The mode calculation function procedure is defined in Appendix C of Akhlaghi and Ichikawa (2015, ApJS 220, 1. arXiv:1505.01664). -- Function: float gal_statistics_mode_value_from_sym (float ‘*sorted’, size_t ‘size’, size_t ‘modeindex’, float ‘sym’) It happens that you have the symmetricity and you want the flux value at that point, this function will do that job. The mode calculation function procedure is defined in Appendix C of Akhlaghi and Ichikawa (2015, ApJS 220, 1. arXiv:1505.01664). -- Function: void gal_statistics_mode_index_in_sorted (float ‘*sorted’, size_t ‘size’, float ‘errorstdm’, size_t ‘*modeindex’, float ‘*modesym’) Find the quantile of the mode of a sorted distribution. The return value is either ‘0’ (not accurate) or ‘1’ (accurate). The mode calculation function procedure is defined in Appendix C of Akhlaghi and Ichikawa (2015, ApJS 220, 1. arXiv:1505.01664).  File: gnuastro.info, Node: Multithreaded programming, Next: Text table into a C array, Prev: Statistical operations, Up: Gnuastro library 10.2.12 Multithreaded programming (‘threads.h’) ----------------------------------------------- In modern times, newer CPU generations don’t have significantly higher frequencies any more. However, CPUs are being manufactured with more cores, enabling more than one operation (thread) at each instant. This can be very useful to speed up many aspects of processing and in particular image processing. Most of the programs in Gnuastro utilize multi-threaded programming for the CPU intensive processing steps. This can potentially lead to a significant decrease in the running time of a program, see *note A note on threads::. In terms of reading the code, you don’t need to know anything about multi-threaded programming. You can simply follow the case where only one thread is to be used. In these cases, threads are not used and can be completely ignored. At the time K&R’s book was written, using threads was not common, so C’s threading capabilities aren’t introduced there. We use POSIX threads for multi-threaded programming, defined in the ‘pthread.h’ system wide header. There are various resources for learning to use POSIX threads, the excellent tutorial from LLNL (https://computing.llnl.gov/tutorials/pthreads/) is a very good start. The book ‘Advanced programming in the Unix environment’(1), by Richard Stevens and Stephen Rago, Addison-Wesley, 2013 (Third edition) also has two chapters explaining the POSIX thread constructs which can be very helpful. An alternative to POSIX threads was OpenMP, but POSIX threads are low level, allowing much more control, while being easier to understand, see *note Why C::. All the situations where threads are used are completely independent with minimal need of coordination between the threads. Such problems are known as “embarrassingly parallel†problems. They are some of the simplest problems to solve with threads and also the ones that benefit most from threads, see the LLNL introduction(2). One very useful POSIX thread concept is ‘pthread_barrier’. Unfortunately, it is only an optional feature in the POSIX standard, so some operating systems don’t include it. Therefore in *note Implementation of pthread_barrier::, we introduce our own implementation. You can ignore this section if your system has this construct. Following that, we describe the helper functions in this header that can greatly simplify writing a multi-threaded program, see *note Gnuastro's thread related functions:: for more. * Menu: * Implementation of pthread_barrier:: Some systems don’t have pthread_barrier * Gnuastro's thread related functions:: Functions for managing threads. ---------- Footnotes ---------- (1) Don’t let the title scare you! The two chapters on Multi-threaded programming are very self-sufficient and don’t need any more knowledge than K&R. (2)  File: gnuastro.info, Node: Implementation of pthread_barrier, Next: Gnuastro's thread related functions, Prev: Multithreaded programming, Up: Multithreaded programming 10.2.12.1 Implementation of ‘pthread_barrier’ ............................................. One optional feature of the POSIX Threads standard is the ‘pthread_barrier’ concept. It is a very useful high-level construct that allows for independent threads to “wait†behind a “barrier†for the rest after they finish. Barriers can thus greatly simplify the code in a multi-threaded program, so they are heavily used in Gnuastro. However, since its an optional feature in the POSIX standard, some operating systems don’t include it. So to make Gnuastro portable, we have written our own implementation of those ‘pthread_barrier’ functions. At ‘./configure’ time, Gnuastro will check if ‘pthread_barrier’ constructs are available on your system or not. If ‘pthread_barrier’ is not available, our internal implementation will be compiled into the Gnuastro library and the definitions and declarations below will be usable in your code with ‘#include ’. -- Type: pthread_barrierattr_t Type to specify the attributes of a POSIX threads barrier. -- Type: pthread_barrier_t Structure defining the POSIX threads barrier. -- Function: int pthread_barrier_init (pthread_barrier_t ‘*b’, pthread_barrierattr_t ‘*attr’, unsigned int ‘limit’) Initialize the barrier ‘b’, with the attributes ‘attr’ and total ‘limit’ (a number of) threads that must wait behind it. This function must be called before spinning off threads. -- Function: int pthread_barrier_wait (pthread_barrier_t ‘*b’) This function is called within each thread, just before it is ready to return. Once a thread’s function hits this, it will “wait†until all the other functions are also finished. -- Function: int pthread_barrier_destroy (pthread_barrier_t ‘*b’) Destroy all the information in the barrier structure. This should be called by the function that spinned-off the threads after all the threads have finished. *Destroy a barrier before re-using it:* It is very important to destroy the barrier before (possibly) reusing it. This destroy function not only destroys the internal structures, it also waits (in 1 microsecond intervals, so you will not notice!) until all the threads don’t need the barrier structure any more. If you immediately start spinning off new threads with a not-destroyed barrier, then the internal structure of the remaining threads will get mixed with the new ones and you will get very strange and apparently random errors that are extremely hard to debug.  File: gnuastro.info, Node: Gnuastro's thread related functions, Prev: Implementation of pthread_barrier, Up: Multithreaded programming 10.2.12.2 Gnuastro’s thread related functions ............................................. These are some high-level functions in ‘gnuastro/threads.h’ to facilitate programming in with POSIX threads. We have created a simple C program for testing these functions in ‘tests/lib/multithread.c’. This small program was compiled and run on your system when you ran ‘make check’. You can use it as a template to easily create small multi-threaded programs and efficiently use your powerful CPU. -- Macro: GAL_THREADS_NON_THRD_INDEX This value will be used in the output of ‘gal_threads_dist_in_threads’ as a non-index. It plays the same role as a string’s null character: ‘‘\0’’: as soon as the parser sees this value, it will stop continuing. -- Function: void gal_threads_attr_barrier_init (pthread_attr_t ‘*attr’, pthread_barrier_t ‘*b’, size_t ‘limit’) Initialize the general thread attribute ‘attr’ and the barrier ‘b’ with ‘limit’ threads to wait behind the barrier. For maximum efficiency, the threads initialized with this function will be detached. Therefore no communication is possible between these threads and in particular ‘pthread_join’ won’t work on these threads. You have to use the barrier constructs to wait for all threads to finish. -- Function: void gal_threads_dist_in_threads (size_t ‘numactions’, size_t ‘numthreads’, size_t ‘**outthrds’, size_t ‘*outthrdcols’) Identify the “indexâ€es (starting from 0) of the actions to be done on each thread in the ‘outthrds’ array. ‘outthrds’ is treated as a 2D array with ‘numthreads’ rows and ‘outthrdcols’ columns. The indexs in each row, identify the actions that should be done by one thread. Please see the explanation below to understand the purpose of this operation. Let’s assume you have $A$ actions (where there is only one function and the input values differ for each action) and $T$ threads available to the system with $A>T$ (common values for these two would be $A>1000$ and $T<10$). Spinning off a thread is not a cheap job and requires a significant number of CPU cycles. Therefore, creating $A$ threads is not the best way to address such a problem. The most efficient way to manage the actions is such that only $T$ threads are created, and each thread works on a list of actions identified for it in series (one after the other). This way your CPU will get all the actions done with minimal overhead. The purpose of this function is to do do what we explained above: each row in the ‘outthrds’ array contains the indexs of actions which must be done by one thread. ‘outthrds’ contains ‘outthrdcols’ columns. In using ‘outthrds’, you don’t have to know the number of columns. The ‘GAL_THREADS_NON_THRD_INDEX’ macro has a role very similar to a string’s ‘\0’: every row finishes with this macro, so can easily stop parsing the indexes in the row when you confront it. Please see the example program in ‘tests/lib/multithread.c’ for a demonstration.  File: gnuastro.info, Node: Text table into a C array, Next: World Coordinate System, Prev: Multithreaded programming, Up: Gnuastro library 10.2.13 Text table into a C array (‘txtarray.h’) ------------------------------------------------ One of the most common formats to store and transfer normally sized data are ASCII files (which can be seen on a text editor). During your processing experiments (with the data, or what programmers call “developingâ€) you will also often want to see how your data is being processed and one of the easiest ways to check out your arrays is to write them out as an ASCII file and check them. The functions here are mainly focused on tables that contain numbers. -- Macro: GAL_TXTARRAY_LOG When an element of the input table cannot be read as a number, the column and row number of the element are stored along with the element into one row of a log file. This macro contains the name of the log-file. -- Function: void gal_txtarray_txt_to_array (char ‘*filename’, double ‘**array’, size_t ‘*s0’, size_t ‘*s1’) Store the ASCII text table in ‘filename’ into the C array ‘array’ which has ‘s0’ rows and ‘s1’ columns. Any blank lines or lines starting with ‘#’ (comments) will be ignored. The column delimiters (separating one column from the previous and next) are ‘‘ ’’ (space), ‘‘,’’, ‘TAB’. -- Function: void gal_txtarray_printf_format (int ‘numcols’, char ‘**fmt’, int ‘*int_cols’, int ‘*accu_cols’, int ‘*space’, int ‘*prec’, char ‘forg’) Return the ‘printf’ formatting string (‘fmt’) for ‘numcols’ columns. Three types of output columns are assumed: integers, normal accuracy floating points and extra-precision floating points. Normally most columns will not need too much accuracy when printing (for example only 3 decimals might be enough). However usually a very limited number of columns will need more precision (like RA and Dec). So to store space (each character is a byte) and also make the table more readable, we allow these two types of floating points. ‘int_cols’ and ‘accu_cols’ are arrays containing the column numbers (starting from zero) that contain integers and extra-accuracy columns. The ending of the column indexes in ‘int_cols’ and ‘accu_cols’ is defined by a negative number. ‘space’ is a three element array which will keep the number of characters that must be used for the integer, normal-accuracy and extra-accuracy columns. ‘prec’ is a two element array which contains the number of decimals to print for the normal and extra accuracy columns. ‘forg’ (read as ‘f-or-g’) is the ‘printf’ type for the floating point numbers: either ‘f’ (as in ‘%f’, which will only print decimals) and ‘g’ (as in ‘%g’, for either printing decimals or exponentials). See ‘gal_txtarray_array_to_txt’ for more. -- Function: void gal_txtarray_array_to_txt (double ‘*array’, size_t ‘s0’, size_t ‘s1’, char ‘*comments’, int ‘*int_cols’, int ‘*accu_cols’, int ‘*space’, int ‘*prec’, char ‘forg’, const char ‘*filename’) Print the C array ‘array’ (with ‘s0’ rows and ‘s1’ columns) as an ASCII text table in ‘filename’. The string pointed to by ‘comments’ will be printed at the top of the table. See the explanation of ‘gal_txtarray_printf_format’ for the other arguments.  File: gnuastro.info, Node: World Coordinate System, Prev: Text table into a C array, Up: Gnuastro library 10.2.14 World Coordinate System (‘wcs.h’) ----------------------------------------- The FITS world coordinate system is a mechanism to give physical values to the data points. In the case of images, it can be used to convert pixel images to celestial coordinates like the right ascension and declination. Gnuastro doesn’t have any functions to actually do the transformations, the standard tool for doing this in astronomy is WCSLIB (see *note WCSLIB::). The functions introduced here are just wrappers around the lower-level functions provided by WCSLIB. -- Function: void gal_wcs_xy_array_to_radec (struct wcsprm ‘*wcs’, double ‘*xy’, double ‘*radec’, size_t ‘number’, size_t ‘stride’) Convert the image coordinates ‘xy’ (a two column array with ‘number’ rows) to world coordinates ‘wcs’ (also a two column array, which has to have been allocated prior to this function) using the conversion parameters in ‘wcs’. ‘stride’ is the number of columns in a larger array, see below. It might happen that you have one array which contains both the image and world coordinates along with many more columns. ‘stride’ is the width of that larger array. If such an array doesn’t exist and ‘xy’ and ‘radec’ are separately allocated arrays with $2\times$‘number’ elements, then just set the value of ‘stride’ to ‘2’. -- Function: void gal_wcs_radec_array_to_xy (struct wcsprm ‘*wcs’, double ‘*radec’, double ‘*xy’, size_t ‘number’, size_t ‘stride’) Similar to ‘gal_wcs_xy_array_to_radec’ but convert the world coordinates in ‘radec’ to image coordinates in ‘xy’. -- Function: double gal_wcs_angular_distance_deg (double ‘r1’, double ‘d1’, double ‘r2’, double ‘d2’) Return the angular distance (in degrees) between a point located at (‘r1’, ‘d1’) to (‘r2’, ‘d2’). All input coordinates are in degrees. The distance (along a great circle) on a sphere between two points is calculated with the equation below. Since the pixel sides are usually very small, we won’t be using the direct formula: $$\cos(d)=\sin(d_1)\sin(d_2)+\cos(d_1)\cos(d_2)\cos(r_1-r_2)$$ Here, we will be using the Haversine formula (https://en.wikipedia.org/wiki/Haversine_formula) which is better considering floating point errors: $${\sin^2(d)\over 2}=\sin^2\left( {d_1-d_2\over 2} \right)+\cos(d_1)\cos(d_2)\sin^2\left( {r_1-r_2\over 2} \right)$$ -- Function: void gal_wcs_pixel_scale_deg (struct wcsprm ‘*wcs’, double ‘*dx’, double ‘*dy’) Return the pixel scale of the WCS structure ‘wcs’ for the two image dimensions ‘dx’ and ‘dy’ in degrees. Here, the X-axis is the first FITS axis, or the horizontal axis when viewed in SAO ds9. -- Function: double gal_wcs_pixel_area_arcsec2 (struct wcsprm ‘*wcs’) Given the WCS structure ‘wcs’ calculate the pixel area in arcsec-squared.  File: gnuastro.info, Node: Developing, Next: Gnuastro programs list, Prev: Libraries, Up: Top 11 Developing ************* The basic idea of GNU Astronomy Utilities is for an interested astronomer to be able to easily understand the code of any of the programs or libraries, be able to modify the code if s/he feels there is an improvement and finally, to be able to add new programs or libraries for their own benefit, and the larger community if they are willing to share it. In short, we hope that at least from the software point of view, the “obscurantist faith in the expert’s special skill and in his personal knowledge and authority†can be broken, see *note Science and its tools::. The following software architecture can be one of the most basic and easy to understand for any interested inquirer. In this chapter, first some general design choices are tackled in ‘Why C’ and ‘Program design philosophy’. The project management webpage and mailing lists are explained in *note Gnuastro project webpage:: and ‘Developing mailing lists’. In *note Coding conventions::, Gnuastro’s adopted coding conventions are discussed and is followed by *note Program source:: which describes how to easily navigate the source files in each program and also contains a template program to easily add new programs. Some other general aspects are then discussed: *note Documentation::, *note Building and debugging::, *note Test scripts::, and *note Developer's checklist::. This chapter finishes with a full description of Gnuastro’s work-flow in *note Contributing to Gnuastro::. * Menu: * Why C:: Why Gnuastro is designed in C. * Program design philosophy:: General ideas behind the package structure. * Gnuastro project webpage:: Central hub for Gnuastro activities. * Developing mailing lists:: Stay up to date with Gnuastro’s development. * Coding conventions:: Gnuastro coding conventions. * Program source:: Conventions for the code. * Documentation:: Documentation is an integral part of Gnuastro. * Building and debugging:: Build and possibly debug during development. * Test scripts:: Understanding the test scripts. * Developer's checklist:: Checklist to finalize your changes. * Contributing to Gnuastro:: Share your changes with all users.  File: gnuastro.info, Node: Why C, Next: Program design philosophy, Prev: Developing, Up: Developing 11.1 Why C programming language? ================================ Currently the programming language that is most commonly used in scientific applications is C++, and more recently Python. One of the main reasons behind this choice is that through the Object oriented programming paradigm, they offer a much higher level of abstraction. However, GNU Astronomy Utilities are written in the C programming language. The reasons can be summarized with simplicity, portability and speed. All three are very important in a scientific software. Simplicity can best be demonstrated in a comparison of the main books of C++ and C. The “C programming languageâ€(1) book, written by the authors of C, is only 286 pages and covers a very good fraction of the language, it has also remained unchanged from 1988. C is the main programming language of nearly all operating systems and there is no plan of any significant update. On the other hand, the most recent “C++ programming languageâ€(2) book, also written by its author, has 1366 pages and its fourth edition came out in 2013! As discussed in *note Science and its tools::, it is very important for other scientists to be able to readily read the code of a program at their will with minimum requirements. In C++, inheriting objects in the object oriented programming paradigm and their internal functions make the code very easy to write for the programmer who is deeply invested in those objects and understands all their relations well. But it simultaneously makes reading the program for a first time reader (a curious scientist who wants to know only how a small step was done) extremely hard. Before understanding the methods, the scientist has to invest a lot of time in understanding those objects and their relations. But in C all variables can be given as the basic language types for example ‘int’s or ‘float’s and their pointers to define arrays. So when an outside reader is only interested in one part of the program, that part is all they have to understand. Recently it is also becoming common to write scientific software in Python, or a combination of it with C or C++. Python is a high level scripting language which doesn’t need compilation. It is very useful when you want to do something on the go and don’t want to be halted by the troubles of compiling, linking, memory checking, etc. When the data sets are small and the job is temporary, this ability of Python is great and is highly encouraged. A very good example might be plotting, in which Python is undoubtedly one of the best. But as the data sets increase in size and the processing becomes very complicated, the speed of Python scripts significantly decrease. So when the program doesn’t change too often and is widely used in a large community mostly on large data sets (like astronomical images), using Python will waste a lot of valuable research-hours. It is possible to wrap C or C++ functions with Python to fix the speed issue. Like C++, Python is object oriented, so as explained above, it needs a high level of experience with that particular program to fully understand its inner workings. To make things worse, since it is mainly for fast and on the go programming, it can undergo significant changes. One recent example is how Python 2.x and Python 3.x are not compatible. Lots of research teams that invested heavily in Python 2.x cannot benefit from Python 3.x or future versions any more. Some converters are available, but since they are automatic, lots of complications might arise in the conversion. Thus, re-writing all the changes would be the only truly reliable option. If a research project begins using Python 3.x today, there is no telling how compatible their investments will be when Python 4.x or 5.x will come out. This stems from the core principles of Python, which are very useful when you look in the ‘on the go’ basis as described before and not future usage. Future-proof code (as long as current operating systems will be used) will be written in C. The portability of C is best demonstrated by the fact that both C++ and Python are part of the C-family of programming languages which also include Java, Perl, and many other languages. C libraries can be immediately included in C++ and with it is easily possible to write wrappers for C libraries in programs in all C-family programming languages. This will allow other scientists to benefit from C libraries with any of those languages. With version 0.2, Gnuastro’s C library is installed along with the programs and task 13786(3) has been defined to add wrappers for higher level languages. The final reason was speed. This is another very important aspect of C which is not independent of simplicity (first reason discussed above). The abstractions provided by the higher-level languages (which also makes learning them harder for a newcomer) comes at the cost of speed. Since C is a low-level language(4) (closer to the hardware), it is much less complex for both the human reader and the computer. The former was discussed above in simplicity and the latter helps in making the program run more efficiently (faster). This thus allows for a closer relation between the scientist/programmer (program) and the actual data/processing. The GNU coding standards(5) also encourage the use of C over all other languages when generality of usage and “high speed†is desired. ---------- Footnotes ---------- (1) Brian Kernighan, Dennis Ritchie. _The C programming language_. Prentice Hall, Inc., Second edition, 1988. It is also commonly known as K&R and is based on the ANSI C and ISO C90 standards. (2) Bjarne Stroustrup. _The C++ programming language_. Addison-Wesley Professional; 4 edition, 2013. (3) (4) Low-level languages are those that directly operate the hardware like assembly languages. So C is actually a high-level language, but it can be considered one of the lowest-level, high-level languages. (5)  File: gnuastro.info, Node: Program design philosophy, Next: Gnuastro project webpage, Prev: Why C, Up: Developing 11.2 Program design philosophy ============================== The core processing functions of each program are written mostly with the basic ISO C90 standard. We do make lots of use of the GNU additions to the C language in the GNU C library, but these additional functions are mainly used in the user interface functions (reading your inputs and preparing them prior to or after the analysis). The actual algorithms, which most scientists would be more interested in, are much more closer to ISO C90. For this reason, the source files containing user interface code and those containing actual processing code are clearly separated, see *note Program source::. If anything particular to the GNU C library is used in the processing functions, it is explained in the comments in between the code. Similar to GNU Coreutils, all the Gnuastro programs provide very low level operations. This enables you to use the GNU Bash scripting language (which is the default in most GNU/Linux operating systems) or any other shell you might be using to operate on a large number of files or do very complex things through the creative combinations of these tools that the authors had never dreamed of. We have put a few simple examples in *note Tutorials::. For example all the analysis output is provided as ASCII tables which you can feed into your favorite plotting program to inspect visually. Python’s Matplotlib is very useful for fast plotting of the tables to immediately check your results. If you want to include the plots in a document, you can use the PGFplots package within LaTeX, no attempt is made to include such operations in Gnuastro. In short, Bash can act as a glue to connect the inputs and outputs of all these various Gnuastro programs (and other programs) in any fashion you please. The advantage of this architecture is that the programs become small and transparent: the starting and finishing point of every program is clearly demarcated. For nearly all operations on a modern computer, the read/write speed is very insignificant compared to the actual processing a program does. Therefore the complexity which arises from sharing memory in a large application is simply not worth the speed gain. This basic design is influenced by Eric Raymond’s “The Art of Unix Programmingâ€(1) which beautifully describes the design philosophy and practice which lead to the success of Unix-based operating systems(2). ---------- Footnotes ---------- (1) Eric S. Raymond, 2004, _The Art of Unix Programming_, Addison-Wesley Professional Computing Series. (2) KISS principle: Keep It Simple, Stupid!  File: gnuastro.info, Node: Gnuastro project webpage, Next: Developing mailing lists, Prev: Program design philosophy, Up: Developing 11.3 Gnuastro project webpage ============================= Gnuastro’s central management hub (https://savannah.gnu.org/projects/gnuastro/)(1) is located on GNU Savannah (https://savannah.gnu.org/)(2). It is the central software development management system for all GNU projects. Through this central hub, you can view the list of activities that the developers are engaged in, their activity on the version controlled source, and other things. Each defined activity in the development cycle is known as an ‘issue’ (or ‘item’). An issue can be a bug (see *note Report a bug::), or a suggested feature (see *note Suggest new feature::) or an enhancement or generally any _one_ job that is to be done. In Savannah, issues are classified into three categories or ‘tracker’s: Support This tracker is a way that (possibly anonymous) users can get in touch with the Gnuastro developers. It is a complement to the bug-gnuastro mailing list (see *note Report a bug::). Anyone can post an issue to this tracker. The developers will not submit an issue to this list. They will only reassign the issues in this list to the other two trackers if they are valid(3). Ideally (when the developers have time to put on Gnuastro, please don’t forget that Gnuastro is a volunteer effort), there should be no open items in this tracker. Bugs This tracker contains all the known bugs in Gnuastro (problems with the existing tools). Tasks The items in this tracker contain the future plans (or new features/capabilities) that are to be added to Gnuastro. All the trackers can be browsed by a (possibly anonymous) visitor, but to edit and comment on the Bugs and Tasks trackers, you have to be a registered Gnuastro developer. When posting an issue to a tracker, it is very important to choose the ‘Category’ and ‘Item Group’ options accurately. The first contains a list of all Gnuastro’s programs along with ‘Installation’, ‘New program’ and ‘Webpage’. The “Item Group†contains the nature of the issue, for example if it is a ‘Crash’ in the software (a bug), or a problem in the documentation (also a bug) or a feature request or an enhancement. The set of horizontal links on the top of the page (Starting with ‘Main’ and ‘Homepage’ and finishing with ‘News’) are the easiest way to access these trackers (and other major aspects of the project) from any part of the project webpage. Hovering your mouse over them will open a drop down menu that will link you to the different things you can do on each tracker (for example, ‘Submit new’ or ‘Browse’). When you browse each tracker, you can use the “Display Criteria†link above the list to limit the displayed issues to what you are interested in. The ‘Category’ and ‘Group Item’ (explained above) are a good starting point. Any new issue that is submitted to any of the trackers, or any comments that are posted for an issue, is directly forwarded to the gnuastro-devel mailing list (, see *note Developing mailing lists:: for more). This will allow anyone interested to be up to date on the over-all development activity in Gnuastro and will also provide an alternative (to Savannah) archiving for the development discussions. Therefore, it is not recommended to directly post an email to this mailing list, but do all the activities (for example add new issues, or comment on existing ones) on Savannah. *Do I need to be a member in Savannah to contribute to Gnuastro?* No. The full version controlled history of Gnuastro is available for anonymous download or cloning. See *note Production workflow:: for a description of Gnuastro’s Integration-Manager Workflow. In short, you can either send in patches, or make your own fork. If you choose the latter, you can push your changes to your own fork and inform us. We will then pull your changes and merge them into the main project. Please see *note Forking tutorial:: for a tutorial. ---------- Footnotes ---------- (1) (2) (3) Some of the issues registered here might be due to a mistake on the user’s side, not an actual bug in the program.  File: gnuastro.info, Node: Developing mailing lists, Next: Coding conventions, Prev: Gnuastro project webpage, Up: Developing 11.4 Developing mailing lists ============================= To keep the developers and interested users up to date with the activity and discussions within Gnuastro, there are two mailing lists which you can subscribe to: ‘gnuastro-devel@gnu.org’ (at ) All the posts made in the support, bugs and tasks discussions of *note Gnuastro project webpage:: are also sent to this mailing address and archived. By subscribing to this list you can stay up to date with the discussions that are going on between the developers before, during and (possibly) after working on an issue. All discussions are either in the context of bugs or tasks which are done on Savannah and circulated to all interested people through this mailing list. Therefore it is not recommended to post anything directly to this mailing list. Any mail that is sent to it from Savannah to this list has a link under the title “Reply to this item at:â€. That link will take you directly to the issue discussion page, where you can read the discussion history or join it. While you are posting comments on the Savannah issues, be sure to update the meta-data. For example if the task/bug is not assigned to anyone and you would like to take it, change the “Assigned to†box, or if you want to report that it has been applied, change the status and so on. All these changes will also be circulated with the email very clearly. ‘gnuastro-commits@gnu.org’ (at ) This mailing list is defined to circulate all commits that are done in Gnuastro’s version controlled source, see *note Version controlled source::. If you have any ideas, or suggestions on the commits, please use the bug and task trackers on Savannah to followup the discussion, do not post to this list. All the commits that are made for an already defined issue or task will state the respective ID so you can find it easily.  File: gnuastro.info, Node: Coding conventions, Next: Program source, Prev: Developing mailing lists, Up: Developing 11.5 Coding conventions ======================= Generally we try our best to follow the GNU coding standards, besides those the following conventions are adhered to until now. If new code is also added in the same manner, it would be much more easily readable by any interested astronomer (who will become familiar with it after reading once). • It is very important that the code be easy to read by the eye. So when the order of several lines within a function does not matter (mostly when defining variables at the start of a function). You should put the lines in the order of increasing length and group the variables with similar types such that this half-pyramid of declarations becomes most visible. If the reader is interested, a simple search will show them the variable they are interested in. However, when looking through the functions or reading the separate steps of the functions, this ‘order’ in the declarations will make reading the rest of the function steps much more easier and pleasant to the eye. • When ever you see that the function cannot be fully displayed (vertically) in your monitor, this is a sign that it has become too long and should be broken up into multiple functions. 40 lines is usually a good reference. When the start and end of a function are clearly visible in one glance, the function is much more easier to understand. This is most important for low-level functions (which usually define a lot of variables). Low-level functions do most of the processing, they will also be the most interesting part of a program for an inquiring astronomer. This convention is less important for higher level functions that don’t define too many variables and whose only purpose is to run the lower-level functions in a specific order and with checks. In general you can be very liberal in breaking up the functions into smaller parts, the GNU Compiler Collection (GCC) will automatically compile the functions as inline functions when the optimizations are turned on. So you don’t have to worry about decreasing the speed. By default Gnuastro will compile with the ‘-O3’ optimization flag. • All Gnuastro hand-written text files (C source code, Texinfo documentation source, and version control commit messages) should not exceed *75* characters per line. Monitors today are certainly much wider, but with this limit, reading the functions becomes much more easier. Also for the developers, it allows multiple files (or multiple views of one file) to be displayed beside each other on wide monitors. Emacs’s buffers are excellent for this capability, setting a buffer width of 80 with ‘’ will allow you to view and work on several files or different parts of one file using the wide monitors common today. Emacs buffers can also be used as a shell prompt and compile the program (with ), and 80 characters is the default width in most terminal emulators. If you use Emacs, Gnuastro sets the 75 character ‘fill-column’ variable automatically for you, see cartouche below. For long comments you can use press in Emacs to separate them into separate lines automatically. For long literal strings, you can use the fact that in C, two strings immediately after each other are concatenated, for example ‘"The first part, " "and the second part."’ Note the space character in the end of the first part. Since they are now separated, you can easily break a long literal string into several lines and adhere to the maximum 75 character line length policy. • The headers required by each source file (ending with ‘.c’) should be defined inside of it. All the headers a program needs should not be stacked in another header to include in all source files (for example ‘main.h’). Although most ‘professional’ programmers choose the latter type, Gnuastro is primarily written for inquisitive astronomers (who are generally amateur programmers). This is very useful for readability by a first time reader. ‘main.h’ may only include the header file(s) that define types that the main program structure needs, see ‘main.h’ in *note Program source::. Those particular header files that are included in ‘main.h’ can of course be ignored (not included) in separate source files. • The headers should be classified (by an empty line) into separate groups: 1. ‘#include ’: This must be the first code line (not commented or blank) in each source file. It sets macros that the GNU Portability Library (Gnulib) will use for the possible additions/modifications to C library headers. 2. The C library (or GNU C library) header files, for example ‘stdio.h’ or ‘errno.h’. 3. Installed library header files, including Gnuastro’s installed headers (for example ‘cfitsio.h’ or ‘gsl/gsl_rng.h’, or ‘gnuastro/fits.h’). 4. Gnuastro’s internal headers (that are not installed), for example ‘commonparams.h’, or Gnulib’s headers (which are also not installed) like ‘nproc.h’. 5. For programs, the ‘main.h’ file (which is needed by the next group of headers). 6. That particular program’s header files, for example ‘mkprof.h’, or ‘noisechisel.h’. As much as order does not matter when you include the header of each group, sort them by length, see above. • All function names, variables, etc should be in lower case. Macros and pre-processor variables should be in upper case. • Regarding naming of exported header files, functions, variables, macros, and library functions, we adopted similar conventions to those used by the GNU Scientific Library (GSL)(1). In particular, in order to avoid clashes with the names of functions and variables coming from other libraries the name-space ‘‘gal_’’ is prefixed to them. GAL stands for _G_NU _A_stronomy _L_ibrary. Ideally ‘‘gnuastro_’’ should have been used, but that is very long. • All installed header files should be in the ‘lib/gnuastro’ directory (under the top Gnuastro source directory). After installation, they will be put in the ‘$prefix/include/gnuastro’ directory (see *note Installation directory:: for ‘$prefix’). Therefore with this convention Gnuastro’s headers can be included in internal (to Gnuastro) and external (a library user) source files with the same line # include Note that unlike the GSL convention, the header file names are not prefixed with a ‘‘gal_’’. If a user manually mixes the Gnuastro (or GSL) headers with other headers, compilation will break because the installed headers depend on each other (the ‘#include’ directive, with the ‘gnuastro/’ directory, above is present in the installed headers too). Therefore the ‘‘gal_’’ prefix to the file names is redundant(2). • All installed functions and variables should also include the base name of the file in which they are defined as prefix, using underscores to separate words(3). The same applies to exported macros, but in upper case. For example in Gnuastro’s top source directory, the prototype of function ‘gal_box_border_from_center’ is in ‘lib/gnuastro/box.h’, and the macro ‘GAL_POLYGON_MAX_CORNERS’ is defined in ‘lib/gnuastro/polygon.h’. To find the header file in the installed directories, replace ‘lib/’ with ‘$prefix/include/’ (see *note Installation directory:: for ‘$prefix’). This is necessary to give any user (who is not familiar with the library structure) the ability to follow the code of a function that is not in the program or library they are reading. This convention does make the function names longer (a little harder to write), but the extra documentation it provides convention plays an important role in Gnuastro and is worth the cost. • There should be no trailing white space in a line. To do this automatically every time you save a file in Emacs, add the following line to your ‘~/.emacs’ file. (add-hook 'before-save-hook 'delete-trailing-whitespace) • There should be no tabs in the indentation(4). • All similar functions are separated by 5 blank lines to be easily seen to be related in a group when parsing the source code by eye. In Emacs you can use . • One group of functions is separated from another with 20 blank lines. In Emacs you can use . Each group of functions has short descriptive title of the functions in that group. This title is surrounded by asterisks (<*>) to make it clearly distinguishable. Such contextual grouping and clear title are very important for easily understanding the code. The last two conventions are not common and might benefit from a short discussion here. With a good experience in advanced text editor operations, to some extent the last two are redundant for a professional developer. However, recall that Gnuastro aspires to be friendly to un-familiar, and un-experienced (in programming) eyes. In other words, as discussed in *note Science and its tools::, we want the code to appear welcoming to someone who is completely new to coding and only has a scientific curiosity. Newcomers to coding and development, who are curious enough to venture into the code, will not be using (or have any knowledge of) advanced text editors. They will see the raw code in the webpage or on a simple text editor (like Gedit) as plain text. Trying to learn and understand a file with dense functions that are all spaced with one or two blank lines can be very taunting for a newcomer. But when they scroll through the file and see clear titles and meaningful spaces for similar functions (less, meaningful density), we are helping them find and focus on the part they are most interested in sooner and easier. *GNU Emacs, the recommended text editor:* GNU Emacs is an extensible and easily customizable text editor which many programmers rely on for developing due to its countless features. Among them, it allows specification of certain settings that are applied to a single file or to all files in a directory and its sub-directories. In order to harmonize code coming from different contributors, Gnuastro comes with a ‘.dir-locals.el’ file which automatically configures Emacs to satisfy most of the coding conventions above when you are using it within Gnuastro’s directories. Thus, Emacs users can readily start hacking into Gnuastro. If you are new to developing, we strongly recommend this editor. Emacs was the first project released by GNU and is still one of its flagship projects. Some resources can be found at: Official manual At . This is a great and very complete manual which is being improved for over 30 years and is the best starting point to learn it. It just requires a little patience and practice, but rest assured that you will be rewarded. If you install Emacs, you also have access to this manual on the command-line with the following command (see *note Info::). $ info emacs A guided tour of emacs At . A short visual tour of Emacs, officially maintained by the Emacs developers. Unofficial mini-manual At . A shorter manual which contains nice animated images of using Emacs. ---------- Footnotes ---------- (1) (2) Note that this applies to GSL’s header files too, for example see ‘eigen/gsl_eigen.h’ in GSL’s source files. GSL uses the ‘gsl_’ filename prefix to separate the headers that will be installed from those that won’t. Therefore this filename prefix a technical internal issue there, which we believe will only confuse the user who doesn’t need to get involved with such issues. (3) The convention to use underscores to separate words, called “snake case†(or “snake_caseâ€). This is also recommended by the GNU coding standards. (4) If you use Emacs, Gnuastro’s ‘.dir-locals.el’ file will automatically never use tabs for indentation. To make this a default in all your Emacs sessions, you can add the following line to your ‘~/.emacs’ file: ‘(setq-default indent-tabs-mode nil)’  File: gnuastro.info, Node: Program source, Next: Documentation, Prev: Coding conventions, Up: Developing 11.6 Program source =================== Besides the fact that all the programs share some functions that were explained in *note Libraries::, everything else about each program is completely independent. In this section the conventions used in all the program sources are explained in *note Mandatory source code files::. To easily understand the explanations in this section you can use *note The TEMPLATE program:: which contains the bare minimum code for one program. This template can also be used to easily add new utilities. * Menu: * Mandatory source code files:: Description of files common to all programs. * The TEMPLATE program:: Template for easy creation of a new program.  File: gnuastro.info, Node: Mandatory source code files, Next: The TEMPLATE program, Prev: Program source, Up: Program source 11.6.1 Mandatory source code files ---------------------------------- Some programs might need lots of source files and if there is no fixed convention, navigating them can become very hard for a new inquirer into the code. The following source files exist in every program’s source directory (which is located in ‘bin/progname’). For small programs, these files are enough. Larger programs will need more files. In general for writing other source files, please choose filenames that are descriptive. ‘main.c’ Each executable has a ‘main’ function, which is located in ‘main.c’. Therefore this file in any program’s source code will be the starting point. No actual processing functions are to be defined in this file, the function(s) in this file are only meant to connect the most high level steps of each program. Generally, ‘main’ will first call the top user interface function to read user input and make all the preparations. Then it will pass control to the top processing function for that program. The functions to do both these jobs must be defined in other source files. ‘main.h’ All the major parameters which will be used in the program must be stored in a structure which is defined in ‘main.h’. The name of this structure is usually ‘prognameparams’, for example ‘imgcropparams’. So ‘#include "main.h"’ will be a staple in all the source codes of the program and most of the functions. Keeping all the major parameters of a program in this structure has the major benefit that most functions will only need one argument: a pointer to this structure. This will significantly facilitate the job of the programmer, the inquirer and the computer. All the programs in Gnuastro are designed to be low-level, small and independent parts, so this structure should not get too large. The main root structure of a program contains at least two other structures: a structure only keeping parameters for user interface functions, which is also defined in ‘main.h’ and the ‘commonparams’ structure which is defined in ‘lib/gnuastro/commonparams.h’(1). The main structure can become very large and since the programmer and inquirer often don’t need to be confused with these parameters mixed with the actual processing parameters, they are conveniently defined in another structure which is named ‘uiparams’ and is also defined in ‘main.h’. It could be defined in ‘ui.h’ (see below) so the main functions remain completely ignorant to it, but its parameters might be needed for reporting input conditions, so it is included as part of the main program structure. This top root structure is conveniently called ‘p’ (short for parameters) by all the programs. The ‘uiparams’ structure is called ‘up’ (for user parameters) and the ‘commonparams’ structure is called ‘cp’. With this convention any reader can immediately understand where to look for the definition of one parameter. With this basic root structure, source code of functions can potentially become full of structure de-reference operators (‘->’) which can make the code very un-readable. In order to avoid this, whenever a parameter is used more than a couple of times in a function, a parameter of the same type and with the same name (so it can be searched) as the desired parameter should be defined and put the value of the root structure inside of it in definition time. For example char *hdu=p->cp.hdu; int verb=p->cp.verb; ‘args.h’ The argument parser structures (which are used by GNU C library’s Argp) for each program are defined in ‘args.h’. They are separate global variables and function definitions that will be used by Argp. We recommend going through the appropriate section in GNU C library to understand their exact meaning, although they should be descriptive and understandable enough by looking at a few of the programs. ‘ui.c, ui.h’ The user interface functions are also a unique set of functions in all the programs, so they are particularly named ‘ui.c’ and ‘ui.h’ in all the programs. Everything related to reading the user input arguments and options, checking the configuration files and checking the consistency of the input parameters before the actual program is run should be done in this file. Since most functions are the same, with only the internal checks and structure parameters differing, we recommend going through several of the examples and structuring your ‘ui.c’ in a similar fashion with the rest of the programs. The most high-level function in ‘ui.c’ is named ‘setparams’ which accepts ‘int argc, char *argv[]’ and a pointer to the root structure for that program, see the explanation for ‘main.h’. This is the function that ‘main’ calls. The basic idea of the functions in this file is that the processing functions should need a minimum number of such checks. With this convention an inquirer who only wants to understand only one part (mostly the processing part and not user input details) of the code can easily do so. It also makes all the errors related to input appear before the processing begins which is more convenient for the user. ‘progname.c’ The main processing functions in each program which keep the function(s) that ‘main()’ will call are in a file named ‘progname.c’, for example ‘imgcrop.c’ or ‘noisechisel.c’. The function within these files which ‘main()’ calls is also named after the program, for example void imgcrop(struct imgcropparams *p) or void noisechisel(struct noisechiselparams *p) In this manner, if an inquirer is interested the processing steps, they can immediately come and check this file for the first processing step without having to go through ‘main.c’ first. In most situations, any failure in any step of the programs will result in an informative error message and an immediate abort in the program. So there is no need for return values. Under more complicated situations where a return value might be necessary, ‘void’ will be replaced with an ‘int’ in the examples above. ‘cite.h’ This file keeps the function to be called if the user runs any of the programs with ‘--cite’, see *note Operating modes::. ---------- Footnotes ---------- (1) ‘lib/gnuastro/commonparams.h’ is a program-specific header and not installed as part of the libraries.  File: gnuastro.info, Node: The TEMPLATE program, Prev: Mandatory source code files, Up: Program source 11.6.2 The TEMPLATE program --------------------------- In the ‘Version controlled source’, the ‘bin/’ directory contains the source code for each program in a separate sub-directory. The ‘bin/TEMPLATE’ directory contains the bare-minimum files to create a new program. It can be used to understand the conventions described in *note Program source::, or to easily create a new program. The extra creativity offered by libraries comes at a cost: you have to actually write your ‘main’ function in the programming language of your choice, and compile it before you can use it. You will also need to find a way to pass input and output information to the function. So when an operation has well-defined inputs and outputs and is commonly needed, it is much more worthwhile to simply do the work in a program (either by modifying an existing one or creating a new one), instead of the using underlying libraries every time. To define your new program based on this template, just take the following steps: 1. Select a name for your new program (for example ‘myprog’). 2. Copy the ‘TEMPLATE’ directory to a directory with your program’s name: $ cp -R bin/TEMPLATE bin/myprog 3. Open ‘configure.ac’ in the top Gnuastro source. This file manages the operations that are done when a user runs ‘./configure’. Going down the file, you will notice repetitive parts for each program. Copy one of those and correct the names of the copied program to your new program name. We follow alphabetic ordering here, so please place it correctly. There are multiple places where this has to be done, so be patient and go down to the bottom of the file. Ultimately add ‘bin/myprog/Makefile’ to ‘AC_CONFIG_FILES’, only here the ordering depends on the length of the name. 4. Open ‘Makefile.am’ in the top Gnuastro source. Similar to the previous step, add your new program similar to all the other programs. 5. Change ‘TEMPLATE’ to ‘myprog’ in the file names and contents of the files in the ‘bin/myprog/’ directory. 6. Run the following command to re-build the configuration and build system. $ autoreconf -f Your new program will be built the next time you run ‘./configure’ and ‘make’.  File: gnuastro.info, Node: Documentation, Next: Building and debugging, Prev: Program source, Up: Developing 11.7 Documentation ================== Documentation (this book) is an integral part of Gnuastro. Documentation is not considered a separate project. So, no change is considered valid for implementation unless the respective parts of the book have also been updated. The following procedure can be a good suggestion to take when you have a new idea and are about to start implementing it. The steps below are not a requirement, the important thing is that when you send the program to be included in Gnuastro, the book and the code have to both be fully up-to-date and compatible and the purpose should be very clearly explained. You can follow any path you choose to do this, the following path was what we found to be most successful during the initial design and implementation steps of Gnuastro. 1. Edit the book and fully explain your desired change, such that your idea is completely embedded in the general context of the book with no sense of discontinuity for a first time reader. This will allow you to plan the idea much more accurately and in the general context of Gnuastro or a particular program. Later on, when you are coding, this general context will significantly help you as a road-map. A very important part of this process is the program introduction, which explains the purposes of the program. Before actually starting to code, explain your idea’s purpose thoroughly in the start of the program section you wish to add or edit. While actually writing its purpose for a new reader, you will probably get some very valuable ideas that you hadn’t thought of before, this has occurred several times during the creation of Gnuastro. If an introduction already exists, embed or blend your idea’s purpose with the existing purposes. We emphasize that doing this is equally useful for you (as the programmer) as it is useful for the user (reader). Recall that the purpose of a program is very important, see *note Program design philosophy::. As you have already noticed for every program, it is very important that the basics of the science and technique be explained in separate subsections prior to the ‘Invoking Programname’ subsection. If you are writing a new program or your addition involves a new concept, also include such subsections and explain the concepts so a person completely unfamiliar with the concepts can get a general initial understanding. You don’t have to go deep into the details, just enough to get an interested person (with absolutely no background) started. If you feel you can’t do that, then you have probably not understood the concept yourself! Have in mind that your only limitation in length is the fatigue of the reader after reading a long text, nothing else. It might also help if you start implementing your idea in the ‘Invoking ProgramName’ subsection (explaining the options and arguments you have in mind) at this stage too. Actually starting to write it here will really help you later when you are coding. 2. After you have finished adding your initial intended plan to the book, then start coding your change or new program within the Gnuastro source files. While you are coding, you will notice that somethings should be different from what you wrote in the book (your initial plan). So correct them as you are actually coding. 3. In the end, read the section in the book that you edited completely and see if you didn’t miss any change in the coding and to see if the context is fairly continuous for a first time reader (who hasn’t seen the book or had known of Gnuastro before you made your change).  File: gnuastro.info, Node: Building and debugging, Next: Test scripts, Prev: Documentation, Up: Developing 11.8 Building and debugging =========================== To build the various programs and libraries in Gnuastro, the GNU build system is used which defines the steps in *note Quick start::. It consists of GNU Autoconf and GNU Automake and GNU Libtool which are collectively known as GNU Autotools. They provide a very portable system to check the environment a program is to be installed on prior to compiling and set the compilation conditions based on the particular user. They also make installing everything in their standard places very easy for the programmer. Most of the small caps files that you see in the top source directory of the tarball are created by these three tools (see *note Version controlled source::). To facilitate the building and testing of your work during development, Gnuastro comes with two scripts: ‘tmpfs-config-make’ and ‘tests/during-dev.sh’. The former is fully described in *note Configure and build in RAM::. During development, you would commonly run this command only once (at the start of your work). The latter is designed to be run each time you make a change and want to test your work (with some possible input and output). The script itself is heavily commented and thoroughly describes the best way to use it, so we won’t repeat it here. As a summary: you specify the build directory, an output directory (for the built program to be run in and also contains the inputs), the program’s short name and the arguments and options that it should be run with. This script will then build Gnuastro, go to the output directory and run the built executable from there. One option for the output directory might be your desktop, so you can easily see the output files and delete them when you are finished. The main purpose of these scripts is to keep your source directory clean and facilitate your development. By default all the programs are compiled with optimization flags for increased speed. A side effect of optimization is that valuable debugging information is lost. All the libraries are also linked as shared libraries by default. Shared libraries further complicate the debugging process and significantly slow down the compilation (the ‘make’ command). So during development it is recommended to configure Gnuastro as follows: $ ./configure --disable-shared CFLAGS="-g -O0" These options to configure are already included in ‘tmpfs-config-make’, you just have to un-comment them. In order to understand the building process, you can go through the Autoconf, Automake and Libtool manuals, like all GNU manuals they provide both a great tutorial and technical documentation. The “A small Hello World†section in Automake’s manual (in chapter 2) can be a good starting guide after you have read the separate introductions.  File: gnuastro.info, Node: Test scripts, Next: Developer's checklist, Prev: Building and debugging, Up: Developing 11.9 Test scripts ================= As explained in *note Tests::, for every program some simple tests are written to check the various independent features of the program. All the tests are placed in the ‘tests/’ directory. There is one script (‘prepconf.sh’) in this folder and several ‘Makefile’s. The script is the first ‘test’ that will be run. It will copy all the configuration files from the various directories to a ‘.gnuastro’ directory which it will make so the various tests can set the default values. For each program, the tests are placed inside directories with the program name. Each test is written as a shell script. The last line of this script is the test which runs the program with certain parameters. The return value of this script determines the fate of the test, see the “Support for test suites†chapter of the Automake manual for a very nice and complete explanation. In every script, two variables are defined at first: ‘prog’ and ‘execname’. The first specifies the program name and the second the location of the executable. The most important thing to have in mind about all the test scripts is that they are run from inside the ‘tests/’ directory in the “build treeâ€. Which can be different from the directory they are stored in (known as the “source treeâ€). The ‘tmpfs-config-make’ script uses this feature (see *note Configure and build in RAM::). This distinction is made by GNU Autoconf and Automake (which configure, build and install Gnuastro) so that you can install the program even if you don’t have write access to the directory keeping the source files. See the “Parallel build trees (a.k.a VPATH builds)†in the Automake manual for a nice explanation. Because of this, any possible data that was not generated by other tests (and is thus in the build tree), for example the catalogs in ImageCrop tests, has a ‘$topsrc’ prefix instead of ‘../’ for the build three. This ‘$topsrc’ variable points to the source tree where the script can find the source data (it is defined in ‘tests/Makefile.am’). The executables and other test products were built in the build tree (where they are being run), so they don’t need to be prefixed with that variable. This is also true for images or files that were produced by other tests.  File: gnuastro.info, Node: Developer's checklist, Next: Contributing to Gnuastro, Prev: Test scripts, Up: Developing 11.10 Developer’s checklist =========================== This is a checklist of things to do after applying your changes/additions in Gnuastro: 1. If the change is non-trivial, write test(s) in the ‘tests/progname/’ directory to test the change(s)/addition(s) you have made. Then add their file names to ‘tests/Makefile.am’. 2. Run ‘$ make check’ to make sure everything is working correctly. 3. Make sure the documentation (this book) is completely up to date with your changes, see *note Documentation::. 4. Commit your change to your issue branch (see *note Production workflow:: and *note Forking tutorial::) Afterwards, run Autoreconf to generate the appropriate version number: $ autoreconf -f 5. Finally, to make sure everything will be built, installed and checked correctly run $ make distcheck This command will create a distribution file (ending with ‘.tar.gz’) and try to compile it in the most general cases, then it will run the tests on what it has built in its own mini-environment. If ‘$ make distcheck’ finishes successfully, then you are safe to send your changes to us to implement or for your own purposes. See *note Production workflow:: and *note Forking tutorial::.  File: gnuastro.info, Node: Contributing to Gnuastro, Prev: Developer's checklist, Up: Developing 11.11 Contributing to Gnuastro ============================== You have this great idea or have found a good fix to a problem which you would like to implement in Gnuastro. You have also become familiar with the general design of Gnuastro in the previous sections of this chapter (see *note Developing::) and want to start working on and sharing your new addition/change with the whole community as part of the official release. This is great and your contribution is most welcome. This section and the next (see *note Developer's checklist::) are written in the hope of making it as easy as possible for you to share your great idea with the Gnuastro community. In this section we discuss the final steps you have to take: legal and technical. From the legal perspective, the copyright of any work you do on Gnuastro has to be assigned to the Free Software Foundation (FSF) and the GNU operating system, or you have to sign a disclaimer. We do this to ensure that Gnuastro can remain free in the future, see *note Copyright assignment::. From the technical point of view, in this section we also discuss commit guidelines (*note Commit guidelines::) and the general version control workflow of Gnuastro in *note Production workflow::, along with a tutorial in *note Forking tutorial::. Recall that before starting the work on your idea, be sure to checkout the bugs and tasks trackers in *note Gnuastro project webpage:: and announce your work there so you don’t end up spending time on something others have already worked on, and also to attract similarly interested developers to help you. * Menu: * Copyright assignment:: Copyright has to be assigned to the FSF. * Commit guidelines:: Guidelines for commit messages. * Production workflow:: Submitting your commits (work) for inclusion. * Forking tutorial:: Tutorial on workflow steps with Git.  File: gnuastro.info, Node: Copyright assignment, Next: Commit guidelines, Prev: Contributing to Gnuastro, Up: Contributing to Gnuastro 11.11.1 Copyright assignment ---------------------------- Gnuastro’s copyright is owned by the FSF. Professor Eben Moglen, of the Columbia University Law School has given a nice summary of the reasons for this at . Below we are copying it verbatim for self consistency (in case you are offline or reading in print). Under US copyright law, which is the law under which most free software programs have historically been first published, there are very substantial procedural advantages to registration of copyright. And despite the broad right of distribution conveyed by the GPL, enforcement of copyright is generally not possible for distributors: only the copyright holder or someone having assignment of the copyright can enforce the license. If there are multiple authors of a copyrighted work, successful enforcement depends on having the cooperation of all authors. In order to make sure that all of our copyrights can meet the record keeping and other requirements of registration, and in order to be able to enforce the GPL most effectively, FSF requires that each author of code incorporated in FSF projects provide a copyright assignment, and, where appropriate, a disclaimer of any work-for-hire ownership claims by the programmer’s employer. That way we can be sure that all the code in FSF projects is free code, whose freedom we can most effectively protect, and therefore on which other developers can completely rely. Please get in touch with the Gnuastro maintainer (currently Mohammad Akhlaghi, akhlaghi -at- gnu -dot- org) to follow the procedures. It is possible to do this for each change (good for for a single contribution), and also more generally for all the changes/additions you do in the future within Gnuastro. So if you have already assigned the copyright of your work on another GNU software to the FSF, it should be done again for Gnuastro. The FSF has staff working on these legal issues and the maintainer will get you in touch with them to do the paperwork. The maintainer will just be informed in the end so your contributions can be merged within the Gnuastro source code. Gnuastro will gratefully acknowledge (see *note Acknowledgments::) all the people who have assigned their copyright to the FSF and have thus helped to guarantee the freedom and reliability of Gnuastro. The Free Software Foundation will also acknowledge your copyright contributions in the Free Software Supporter: which will circulate to a very large community (104,444 people in April 2016). See the archives for some examples and subscribe to receive interesting updates. The very active code contributors (or developers) will also be recognized as project members on the Gnuastro project webpage (see *note Gnuastro project webpage::) and can be given a ‘gnu.org’ email address. So your very valuable contribution and copyright assignment will not be forgotten and is highly appreciated by a very large community. If you are reluctant to sign an assignment, a disclaimer is also acceptable. *Do I need a disclaimer from my university or employer?* It depends on the contract with your university or employer. From the FSF’s ‘/gd/gnuorg/conditions.text’: “If you are employed to do programming, or have made an agreement with your employer that says it owns programs you write, we need a signed piece of paper from your employer disclaiming rights to†Gnuastro. The FSF’s copyright clerk will kindly help you decide, please consult the following email address: “assign -at- gnu -dot- orgâ€.  File: gnuastro.info, Node: Commit guidelines, Next: Production workflow, Prev: Copyright assignment, Up: Contributing to Gnuastro 11.11.2 Commit guidelines ------------------------- To be able to cleanly integrate your work with the other developers, *never commit on the ‘master’ branch* (see *note Production workflow:: for a complete discussion and *note Forking tutorial:: for a cookbook example). In short, leave ‘master’ only for changes you fetch, or pull from the official repository (see *note Synchronizing::). In the Gnuastro commit messages, we strive to follow these standards. Note that in the early phases of Gnuastro’s development, we are experimenting and so if you notice earlier commits don’t satisfy some of the guidelines below, it is because they predate that guideline. Commit title The commits have to start with one short descriptive title. The title is separated from the body with one blank line. Run ‘git log’ to see some of the most recent commit messages as an example. In general, the title should satisfy the following conditions: • It is best for the title to be short, about 60 (or even 50) characters. Most emulated command-line terminals are about 80 characters wide. However, we should also allow for the commit hashes which are printed in ‘git log --oneline’, and also branch names or the graph structure outputs of ‘git log’ which are also commonly used. • The title should not finish with any full-stops or periods (‘<.>’). Commit body The body of the commit message is separated from the title by one empty line. Recall that anyone who has subscribed to ‘gnuastro-commits’ mailing list will get the commit in their email after it has been pushed to ‘master’. People will also read them when they synchronize with the main Gnuastro repository (see *note Synchronizing::). Finally, the commit messages will later be used to update the ‘NEWS’ file on each release. Therefore the commit message body plays a very important role in the development of Gnuastro, so please adhere to the following guidelines. • The body should be very descriptive. Start the commit message body by explaining what changes your commit makes from a user’s perspective (added, changed, or removed options, or arguments to programs or libraries, or modified algorithms, or new installation step, or etc). • Try to explain the committed contents as best as you can. Recall that the readers of your commit message do not necessarily have your current background. After some time you will also forget the context, so this request is not just for others(1). Therefore be very descriptive and explain as much as possible: what the bug/task was, justify the way you fixed it and discuss other possible solutions that you might not have included. For the last item, it is best to discuss them thoroughly as comments in the appropriate section of the code, but only give a short summary in the commit message. Note that all added and removed source code lines will also be circulated in the ‘gnuastro-commits’ mailing list. • Like all other Gnuastro’s text files, the lines in the commit body should not be longer than 75 characters, see *note Coding conventions::. This is to ensure that on standard terminal emulators (with 80 character width), the ‘git log’ output can be cleanly displayed (note that the commit message is indented in the output of ‘git log’). If you use Emacs, Gnuastro’s ‘.dir-locals.el’ file will ensure that your commits satisfy this condition (using ). • When the commit is related to a task or a bug, please include the respective ID (in the format of ‘bug/task #ID’, note the space) in the commit message (from *note Gnuastro project webpage::) for interested people to be able to followup the discussion that took place there. If the commit fixes a bug or finishes a task, the recommended way is to add a line after the body with ‘‘This fixes bug #ID.’’, or ‘‘This finishes task #ID.’’. Don’t assume that the reader has internet access to check the bug’s full description when reading the commit message, so give a short introduction too. ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: Production workflow, Next: Forking tutorial, Prev: Commit guidelines, Up: Contributing to Gnuastro 11.11.3 Production workflow --------------------------- Fortunately ‘Pro Git’ has done a wonderful job in explaining the different workflows in Chapter 5(1) and in particular the “Integration-Manager Workflow†explained there. The implementation of this workflow is nicely explained in Section 5.2(2) under “Forked-Public-Projectâ€. We have also prepared a short tutorial in *note Forking tutorial::. Anything on the master branch should always be tested and ready to be built and used. As described in ‘Pro Git’, there are two methods for you to contribute to Gnuastro in the Integration-Manager Workflow: 1. You can send commit patches by email as fully explained in ‘Pro Git’. This is good for your first few contributions. Just note that raw patches (containing only the diff) do not have any meta-data (author name, date and etc). Therefore will not allow us to fully acknowledge your contributions as an author in Gnuastro: in the ‘AUTHORS’ file and at the start of the PDF book. These author lists are created automatically from the version controlled source. To receive full acknowledgement when submitting a patch, is thus advised to use Git’s ‘format-patch’ tool. See Pro Git’s Public project over email (https://git-scm.com/book/en/v2/Distributed-Git-Contributing-to-a-Project#Public-Project-over-Email) section for a nice explanation. If you would like to get more heavily involved in Gnuastro’s development, then you can try the next solution. 2. You can have your own forked copy of Gnuastro on any hosting site you like (GitHub, GitLab, BitBucket, or etc) and inform us when your changes are ready so we merge them in Gnuastro. This is more suited for people who commonly contribute to the code (see *note Forking tutorial::). In both cases, your commits (with your name and information) will be preserved and your contributions will thus be fully recorded in the history of Gnuastro and in the ‘AUTHORS’ file and this book (second page in the PDF format) once they have been incorporated into the official repository. Needless to say that in such cases, be sure to follow the bug or task trackers (or subscribe to the ‘gnuastro-devel’ mailing list) and contact us before hand so you don’t do something that someone else is already working on. In that case, you can get in touch with them and help the job go on faster, see *note Gnuastro project webpage::. This workflow is currently mostly borrowed from the general recommendations of Git(3) and GitHub. But since Gnuastro is under heavy development currently, these might change and evolve to better suite our needs. ---------- Footnotes ---------- (1) (2) (3)  File: gnuastro.info, Node: Forking tutorial, Prev: Production workflow, Up: Contributing to Gnuastro 11.11.4 Forking tutorial ------------------------ This is a tutorial on the second suggested method that you can submit your modifications in Gnuastro (see *note Production workflow::), which is commonly known as forking. Let’s assume you want to start contributing to Gnuastro and you would like to use GitLab(1) to host your work remotely and share it with other Gnuastro developers once you are ready. You can create an empty repository on your hosting service webpage. If this is your first hosted repository on the webpage, you also have to upload your public SSH key(2) for the ‘git push’ command below to work. Here we’ll assume you use the name ‘janedoe’ to refer to yourself everywhere and that you choose ‘gnuastro-janedoe’ as the name of your Gnuastro fork. Any online hosting service will give you an address (similar to ‘‘git@gitlab.com:’’ below) of the empty repository you have created using their webpage, use that address in the third line below. $ git clone git://git.sv.gnu.org/gnuastro.git $ cd gnuastro $ git remote add janedoe git@gitlab.com:janedoe/gnuastro-janedoe.git $ git push janedoe master The full Gnuastro history is now pushed onto your hosting service and the ‘janedoe’ remote is now also following your ‘master’ branch. If you run ‘git remote show REMOTENAME’ for the ‘origin’ and ‘janedoe’ remotes, you will see their difference: the first has pull access and the second doesn’t. This nicely summarizes the main idea behind this workflow: you push to your remote repository, we pull from it and merge it into ‘master’, then you finalize it by pulling from the main repository. To test (compile) your changes during your work, you will need to bootstrap the version controlled source, see *note Bootstrapping:: for a full description. The process above is only necessary for your first time setup, you don’t need to repeat it. However, please repeat the steps below for each independent issue you intend to work on. Let’s assume you have found a bug in ‘lib/statistics.c’’s median calculating function. You announce it (see *note Report a bug::) so everyone knows you are working on it. However, if it is a very simple, clear/obvious and straightforward bug to fix you can skip this initial announcement. With the commands below, you make a branch, checkout to it, correct the bug, check if it is indeed fixed, add it to the staging area, commit it to the new branch and push it to your hosting service. But before all of them, make sure that you are on the ‘master’ branch and that your ‘master’ branch is up to date with the main Gnuastro repository with the first two commands. $ git checkout master $ git pull $ git checkout -b bug-median-stats # Choose a descriptive name $ emacs lib/statistics.c $ # do your checks here $ git add lib/statistics.c $ git commit $ git push janedoe bug-median-stats Your new branch is now on your hosted repository. Through the respective tacker on Savannah (see *note Gnuastro project webpage::) you can then let the other developers know that your ‘bug-median-stats’ branch is ready. They will pull your work, test it themselves and if it is ready to be merged into the main Gnuastro history, they will merge it into the ‘master’ branch. After that is done, you can simply checkout your local ‘master’ branch and pull all the changes from the main repository. After the pull you can run ‘‘git log’’ as shown below, to see how ‘bug-median-stats’ is merged with master. So you can push all the changes to your hosted repository and delete the branches: $ git checkout master $ git pull $ git log --oneline --graph --decorate --all $ git push janedoe master $ git branch -d bug-median-stats # delete local branch $ git push janedoe --delete bug-median-stats # delete remote branch Just as a reminder, always keep your work on each issue in a separate local and remote branch so work can progress on them independently. After you make your announcement, other people might contribute to the branch before merging it in to ‘master’, so this is very important. Also before starting each issue branch from ‘master’, be sure to run ‘git pull’ in ‘master’ as shown above, to start your branch (work) from the most recent history point and thus simplify the final merging of your work. ---------- Footnotes ---------- (1) See for an evaluation of the major existing repositories. (2) For example see this explanation provided by GitLab: .  File: gnuastro.info, Node: Gnuastro programs list, Next: Other useful software, Prev: Developing, Up: Top Appendix A Gnuastro programs list ********************************* GNU Astronomy Utilities 0.2.33-8a3b, contains the following programs. They are sorted in alphabetical order and followed by their version number. A short description is provided for each program which starts with the executable names in ‘thisfont’ followed by a link to the respective section in parenthesis, see *note Naming convention::. Throughout this book, they are ordered based on their context, please see the book contents for contextual ordering. Arithmetic (‘astarithmetic’, see *note Arithmetic::) For arithmetic operations on multiple (theoretically unlimited) number of datasets (images). It has a large and growing set of arithmetic, mathematical, and even statistical operators (for example ‘+’, ‘-’, ‘*’, ‘/’, ‘sqrt’, ‘log’, ‘min’, ‘average’, ‘median’). ConvertType (‘astconvertt’, see *note ConvertType::) Convert astronomical data files (FITS or IMH) to and from several other standard image and data formats, for example TXT, JPEG, EPS or PDF. Convolve (‘astconvolve’, see *note Convolve::) Convolve (blur or smooth) data with a given kernel in spatial and frequency domain on multiple threads. Convolve can also do de-convolution to find the appropriate kernel to PSF-match two images. CosmicCalculator (‘astcosmiccal’, see *note CosmicCalculator::) Do cosmological calculations, for example the luminosity distance, distance modulus, comoving volume and many more. Header (‘astheader’, see *note Header::) Print and manipulate the header data of a FITS file. ImageCrop (‘astimgcrop’, see *note ImageCrop::) Crop region(s) from an image and stitch several images if necessary. Inputs can be in pixel coordinates or world coordinates. ImageStatistics (‘astimgstat’, see *note ImageStatistics::) Get pixel statistics and save histogram and cumulative frequency plots. ImageWarp (‘astimgwarp’, see *note ImageWarp::) Warp image to new pixel grid. Any projective transformation or Homography can be applied to the input images. MakeCatalog (‘astmkcatalog’, see *note MakeCatalog::) Make catalog of labeled image (output of NoiseChisel). The catalogs are highly customizable and adding new calculations/columns is very straightforward. MakeNoise (‘astmknoise’, see *note MakeNoise::) Make (add) noise to an image, with a large set of random number generators and any seed. MakeProfiles (‘astmkprof’, see *note MakeProfiles::) Make mock 2D profiles in an image. The central regions of radial profiles are made with a configurable 2D Monte Carlo integration. It can also build the profiles on an over-sampled image. NoiseChisel (‘astnoisechisel’, see *note NoiseChisel::) Detect and segment signal in noise. It uses a technique to detect very faint and diffuse, irregularly shaped signal in noise (galaxies in the sky), using thresholds that are below the Sky value, see arXiv:1505.01664 (http://arxiv.org/abs/1505.01664). SubtractSky (‘astsubtractsky’, *note SubtractSky::) Find and subtract sky value by comparing the mode and median on a mesh grid. Table (‘asttable’, *note Table::) Convert FITS binary and ASCII tables into other such tables, print them on the command-line, save them in a plain text file, or get the FITS table information.  File: gnuastro.info, Node: Other useful software, Next: GNU Free Documentation License, Prev: Gnuastro programs list, Up: Top Appendix B Other useful software ******************************** In this appendix the installation of programs and libraries that are not direct Gnuastro dependencies are discussed. However they can be useful for working with Gnuastro. * Menu: * SAO ds9:: Viewing FITS images. * PGPLOT:: Plotting directly in C  File: gnuastro.info, Node: SAO ds9, Next: PGPLOT, Prev: Other useful software, Up: Other useful software B.1 SAO ds9 =========== SAO ds9(1) is not a requirement of Gnuastro, it is a FITS image viewer. So to check your inputs and outputs, it is one of the best options. Like the other packages, it might already be available in your distribution’s repositories. It is already pre-compiled in the download section of its webpage. Once you download it you can unpack and install (move it to a system recognized directory) with the following commands (‘x.x.x’ is the version number): $ tar xf ds9.linux64.x.x.x.tar.gz $ sudo mv ds9 /usr/local/bin Once you run it, there might be a complaint about the Xss library, which you can find in your distribution package management system. You might also get an ‘XPA’ related error. In this case, you have to add the following line to your ‘~/.bashrc’ and ‘~/.profile’ file (you will have to log out and back in again for the latter): export XPA_METHOD=local * Menu: * Viewing multiextension FITS:: Configure SAO ds9 for multiextension images. ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: Viewing multiextension FITS, Prev: SAO ds9, Up: SAO ds9 B.1.1 Viewing multiextension FITS images ---------------------------------------- The FITS definition allows for multiple extensions inside a FITS file, each extension can have a completely independent data set inside of it. If you ordinarily open a multi-extension FITS file with SAO ds9, for example by double clicking on the file or running ‘$ds9 foo.fits’, SAO ds9 will only show you the first extension. To be able to switch between the extensions you have to follow these menus in the SAO ds9 window: File→Open Other→Open Multi Ext Cube and then choose the Multi extension FITS file in your computer’s file structure. The method above is a little tedious to do every time you want view a multi-extension FITS file. Fortunately SAO ds9 also provides options that you can use to specify a particular behavior. One of those options is ‘-mecube’ which opens a FITS image as a multi-extension data cube. So on the command-line, if you run ‘$ds9 -mecube foo.fits’ a small window will also be opened, which allows you to switch between the image extensions that ‘foo.fits’ might have. If ‘foo.fits’ only consists of one extension, then SAO ds9 will open as usual. Just to avoid confusion, note that SAO ds9 does not follow the GNU style of separating long and short options as explained in *note Arguments and options::. In the GNU style, this ‘long’ option should have been called like ‘--mecube’, but SAO ds9 does follow those conventions and has its own. It is really convenient if you set ds9 to always run with the ‘-mecube’ option on your graphical display. On GNOME 3 (the most popular graphic user interface for GNU/Linux systems) you can do this by taking the following steps: • Open your favorite text editor and put the following text in a file that ends with ‘.desktop’, for example ‘saods9.desktop’. The file is very descriptive. [Desktop Entry] Type=Application Version=1.0 Name=SAO ds9 Comment=View FITS images Exec=ds9 -mecube %f Terminal=false Categories=Graphic;FITS; • Copy this file into your local (user) applications directory: $ cp saods9.desktop ~/.local/share/applications/ In case you don’t have the directory, you can make it yourself: $ mkdir -p ~/.local/share/applications/ • The steps above will add SAO ds9 as one of your applications. To make it default for every time you click on a FITS file. Right click on a FITS file and select “Open Withâ€, then go into “Other Application...†and choose “SAO ds9â€. In case you are using GNOME 2 you can take the following steps: right click on a FITS file and choose Properties→Open With→Add button. A list of applications will show up, ds9 might already be present in the list, but don’t choose it because it will run with no options. Below the list is an option “Use a custom commandâ€. Click on it and write the following command: ‘ds9 -mecube’ in the box and click “Addâ€. Then finally choose the command you just added as the default and click the “Close†button.  File: gnuastro.info, Node: PGPLOT, Prev: SAO ds9, Up: Other useful software B.2 PGPLOT ========== PGPLOT is a package for making plots in C. It is not directly needed by Gnuastro, but can be used by WCSLIB, see *note WCSLIB::. As explained in *note WCSLIB::, you can install WCSLIB without it too. It is very old (the most recent version was released early 2001!), but remains one of the main packages for plotting directly in C. WCSLIB uses this package to make plots if you want it to make plots. If you are interested you can also use it for your own purposes. If you want your plotting codes in between your C program, PGPLOT is currently one of your best options. The recommended alternative to this method is to get the raw data for the plots in text files and input them into any of the various more modern and capable plotting tools separately, for example the Matplotlib library in Python or PGFplots in LaTeX. This will also significantly help code readability. Let’s get back to PGPLOT for the sake of WCSLIB. Installing it is a little tricky (mainly because it is so old!). You can download the most recent version from the FTP link in its webpage(1). You can unpack it with the ‘tar xf’ command. Let’s assume the directory you have unpacked it to is ‘PGPLOT’, most probably it is: ‘/home/username/Downloads/pgplot/’. open the ‘drivers.list’ file: $ gedit drivers.list Remove the ‘!’ for the following lines and save the file in the end: PSDRIV 1 /PS PSDRIV 2 /VPS PSDRIV 3 /CPS PSDRIV 4 /VCPS XWDRIV 1 /XWINDOW XWDRIV 2 /XSERVE Don’t choose GIF or VGIF, there is a problem in their codes. Open the ‘PGPLOT/sys_linux/g77_gcc.conf’ file: $ gedit PGPLOT/sys_linux/g77_gcc.conf change the line saying: ‘FCOMPL="g77"’ to ‘FCOMPL="gfortran"’, and save it. This is a very important step during the compilation of the code if you are in GNU/Linux. You now have to create a folder in ‘/usr/local’, don’t forget to replace ‘PGPLOT’ with your unpacked address: $ su # mkdir /usr/local/pgplot # cd /usr/local/pgplot # cp PGPLOT/drivers.list ./ To make the Makefile, type the following command: # PGPLOT/makemake PGPLOT linux g77_gcc It should finish by saying: ‘Determining object file dependencies’. You have done the hard part! The rest is easy: run these three commands in order: # make # make clean # make cpg Finally you have to place the position of this directory you just made into the ‘LD_LIBRARY_PATH’ environment variable and define the environment variable ‘PGPLOT_DIR’. To do that, you have to edit your ‘.bashrc’ file: $ cd ~ $ gedit .bashrc Copy these lines into the text editor and save it: PGPLOT_DIR="/usr/local/pgplot/"; export PGPLOT_DIR LD_LIBRARY_PATH=$LD_LIBRARY_PATH:/usr/local/pgplot/ export LD_LIBRARY_PATH You need to log out and log back in again so these definitions take effect. After you logged back in, you want to see the result of all this labor, right? Tim Pearson has done that for you, create a temporary folder in your home directory and copy all the demonstration files in it: $ cd ~ $ mkdir temp $ cd temp $ cp /usr/local/pgplot/pgdemo* ./ $ ls You will see a lot of pgdemoXX files, where XX is a number. In order to execute them type the following command and drink your coffee while looking at all the beautiful plots! You are now ready to create your own. $ ./pgdemoXX ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: GNU Free Documentation License, Next: Index, Prev: Other useful software, Up: Top Appendix C GNU Free Documentation License ***************************************** Version 1.3, 3 November 2008 Copyright © 2000, 2001, 2002, 2007, 2008 Free Software Foundation, Inc. Everyone is permitted to copy and distribute verbatim copies of this license document, but changing it is not allowed. 0. PREAMBLE The purpose of this License is to make a manual, textbook, or other functional and useful document “free†in the sense of freedom: to assure everyone the effective freedom to copy and redistribute it, with or without modifying it, either commercially or noncommercially. Secondarily, this License preserves for the author and publisher a way to get credit for their work, while not being considered responsible for modifications made by others. This License is a kind of “copyleftâ€, which means that derivative works of the document must themselves be free in the same sense. It complements the GNU General Public License, which is a copyleft license designed for free software. We have designed this License in order to use it for manuals for free software, because free software needs free documentation: a free program should come with manuals providing the same freedoms that the software does. But this License is not limited to software manuals; it can be used for any textual work, regardless of subject matter or whether it is published as a printed book. We recommend this License principally for works whose purpose is instruction or reference. 1. APPLICABILITY AND DEFINITIONS This License applies to any manual or other work, in any medium, that contains a notice placed by the copyright holder saying it can be distributed under the terms of this License. Such a notice grants a world-wide, royalty-free license, unlimited in duration, to use that work under the conditions stated herein. The “Documentâ€, below, refers to any such manual or work. Any member of the public is a licensee, and is addressed as “youâ€. You accept the license if you copy, modify or distribute the work in a way requiring permission under copyright law. A “Modified Version†of the Document means any work containing the Document or a portion of it, either copied verbatim, or with modifications and/or translated into another language. 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The operator of an MMC Site may republish an MMC contained in the site under CC-BY-SA on the same site at any time before August 1, 2009, provided the MMC is eligible for relicensing. ADDENDUM: How to use this License for your documents ==================================================== To use this License in a document you have written, include a copy of the License in the document and put the following copyright and license notices just after the title page: Copyright (C) YEAR YOUR NAME. Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled ``GNU Free Documentation License''. If you have Invariant Sections, Front-Cover Texts and Back-Cover Texts, replace the “with...Texts.†line with this: with the Invariant Sections being LIST THEIR TITLES, with the Front-Cover Texts being LIST, and with the Back-Cover Texts being LIST. If you have Invariant Sections without Cover Texts, or some other combination of the three, merge those two alternatives to suit the situation. If your document contains nontrivial examples of program code, we recommend releasing these examples in parallel under your choice of free software license, such as the GNU General Public License, to permit their use in free software.  File: gnuastro.info, Node: Index, Prev: GNU Free Documentation License, Up: Top Index: Macros, structures and functions *************************************** All Gnuastro library’s exported macros start with ‘GAL_’, and its exported structures and functions start with ‘gal_’. This abbreviation stands for _G_NU _A_stronomy _L_ibrary. The next element in the name is the name of the header which declares or defines them, so to use the ‘gal_array_fset_const’ function, you have to ‘#include ’. See *note Gnuastro library:: for more. The ‘pthread_barrier’ constructs are our implementation and are only available on systems that don’t have them, see *note Implementation of pthread_barrier::. [index] * Menu: * gal_array_dabs_array: Array manipulation. (line 231) * gal_array_dconst_divide: Array manipulation. (line 149) * gal_array_dconst_power: Array manipulation. (line 205) * gal_array_dconst_subtract: Array manipulation. (line 184) * gal_array_ddivide_arrays: Array manipulation. (line 156) * gal_array_ddivide_const: Array manipulation. (line 142) * gal_array_dlog10_array: Array manipulation. (line 225) * gal_array_dlog_array: Array manipulation. (line 219) * gal_array_dmultip_arrays: Array manipulation. (line 134) * gal_array_dmultip_const: Array manipulation. (line 127) * gal_array_dpower_arrays: Array manipulation. (line 212) * gal_array_dpower_const: Array manipulation. (line 198) * gal_array_dsubtract_arrays: Array manipulation. (line 191) * gal_array_dsubtract_const: Array manipulation. (line 177) * gal_array_dsum_arrays: Array manipulation. (line 170) * gal_array_dsum_const: Array manipulation. (line 164) * gal_array_float_copy: Array manipulation. (line 50) * gal_array_float_copy_noalloc: Array manipulation. (line 57) * gal_array_fmultip_const: Array manipulation. (line 107) * gal_array_freplace_nonnans: Array manipulation. (line 78) * gal_array_freplace_value: Array manipulation. (line 70) * gal_array_fset_const: Array manipulation. (line 64) * gal_array_fsum_arrays: Array manipulation. (line 120) * gal_array_fsum_const: Array manipulation. (line 114) * gal_array_long_init: Array manipulation. (line 29) * gal_array_long_init_on_region: Array manipulation. (line 36) * gal_array_no_nans: Array manipulation. (line 85) * gal_array_no_nans_double: Array manipulation. (line 95) * gal_array_uchar_copy: Array manipulation. (line 43) * gal_array_uchar_init_on_region: Array manipulation. (line 19) * gal_array_uchar_replace: Array manipulation. (line 100) * gal_box_border_from_center: Bounding box. (line 22) * gal_box_ellipse_in_box: Bounding box. (line 11) * gal_box_overlap: Bounding box. (line 30) * gal_fits_add_to_key_ll: FITS functions. (line 125) * gal_fits_add_to_key_ll_end: FITS functions. (line 141) * gal_fits_add_wcs_to_header: FITS functions. (line 164) * gal_fits_array_to_file: FITS functions. (line 237) * gal_fits_atof_correct_wcs: FITS functions. (line 251) * gal_fits_bitpix_to_datatype: FITS functions. (line 39) * gal_fits_blank_to_value: FITS functions. (line 83) * GAL_FITS_BYTE_BLANK: FITS macros and data structures. (line 12) * gal_fits_change_type: FITS functions. (line 90) * gal_fits_datatype_alloc: FITS functions. (line 71) * gal_fits_datatype_blank: FITS functions. (line 63) * gal_fits_datatype_size: FITS functions. (line 77) * GAL_FITS_DOUBLE_BLANK: FITS macros and data structures. (line 18) * gal_fits_file_name_in_keywords: FITS functions. (line 151) * gal_fits_file_or_ext_name: FITS functions. (line 274) * gal_fits_file_to_double: FITS functions. (line 311) * gal_fits_file_to_float: FITS functions. (line 296) * gal_fits_file_to_long: FITS functions. (line 322) * GAL_FITS_FLOAT_BLANK: FITS macros and data structures. (line 17) * gal_fits_hdu_to_array: FITS functions. (line 227) * gal_fits_img_bitpix_size: FITS functions. (line 53) * GAL_FITS_INT_BLANK: FITS macros and data structures. (line 19) * gal_fits_io_error: FITS functions. (line 12) * GAL_FITS_LLONG_BLANK: FITS macros and data structures. (line 16) * GAL_FITS_LOGICAL_BLANK: FITS macros and data structures. (line 13) * GAL_FITS_LONG_BLANK: FITS macros and data structures. (line 15) * gal_fits_name_is_fits: FITS functions. (line 23) * gal_fits_num_hdus: FITS functions. (line 98) * gal_fits_prep_float_kernel: FITS functions. (line 332) * gal_fits_read_hdu: FITS functions. (line 104) * gal_fits_read_keywords: FITS functions. (line 112) * gal_fits_read_wcs: FITS functions. (line 216) * gal_fits_read_wcs_from_pointer: FITS functions. (line 195) * GAL_FITS_SBYTE_BLANK: FITS macros and data structures. (line 20) * GAL_FITS_SHORT_BLANK: FITS macros and data structures. (line 14) * GAL_FITS_STRING_BLANK: FITS macros and data structures. (line 11) * gal_fits_suffix_is_fits: FITS functions. (line 30) * gal_fits_table_size: FITS functions. (line 261) * gal_fits_table_type: FITS functions. (line 268) * gal_fits_tform_to_datatype: FITS functions. (line 45) * GAL_FITS_UINT_BLANK: FITS macros and data structures. (line 21) * GAL_FITS_ULONG_BLANK: FITS macros and data structures. (line 23) * gal_fits_update_keys: FITS functions. (line 173) * GAL_FITS_USHORT_BLANK: FITS macros and data structures. (line 22) * gal_fits_write_keys_version: FITS functions. (line 182) * gal_git_describe: Git wrappers. (line 15) * GAL_GNUASTRO_HAVE_LIBGIT2: Installation information. (line 25) * GAL_GNUASTRO_HAVE_PTHREAD_BARRIER: Installation information. (line 32) * GAL_GNUASTRO_VERSION: Installation information. (line 14) * gal_linkedlist_add_to_fll: Linked lists. (line 77) * gal_linkedlist_add_to_osll: Linked lists. (line 319) * gal_linkedlist_add_to_sll: Linked lists. (line 254) * gal_linkedlist_add_to_stll: Linked lists. (line 194) * gal_linkedlist_add_to_tdll: Linked lists. (line 140) * gal_linkedlist_add_to_tosll_end: Linked lists. (line 376) * gal_linkedlist_fll_to_array: Linked lists. (line 100) * gal_linkedlist_free_fll: Linked lists. (line 110) * gal_linkedlist_free_fll_array: Linked lists. (line 119) * gal_linkedlist_free_sll: Linked lists. (line 296) * gal_linkedlist_free_tdll: Linked lists. (line 176) * gal_linkedlist_num_int_dll: Linked lists. (line 158) * gal_linkedlist_num_in_fll: Linked lists. (line 94) * gal_linkedlist_num_in_sll: Linked lists. (line 271) * gal_linkedlist_num_in_stll: Linked lists. (line 234) * gal_linkedlist_osll_into_sll: Linked lists. (line 335) * gal_linkedlist_pop_from_fll: Linked lists. (line 86) * gal_linkedlist_pop_from_osll: Linked lists. (line 326) * gal_linkedlist_pop_from_sll: Linked lists. (line 263) * gal_linkedlist_pop_from_stll: Linked lists. (line 210) * gal_linkedlist_pop_from_tdll: Linked lists. (line 149) * gal_linkedlist_pop_from_tosll_start: Linked lists. (line 387) * gal_linkedlist_print_fll_array: Linked lists. (line 69) * gal_linkedlist_print_sll: Linked lists. (line 277) * gal_linkedlist_print_stll: Linked lists. (line 227) * gal_linkedlist_print_tosll: Linked lists. (line 368) * gal_linkedlist_reverse_stll: Linked lists. (line 218) * gal_linkedlist_sll_to_array: Linked lists. (line 284) * gal_linkedlist_smallest_tosll: Linked lists. (line 400) * gal_linkedlist_tdll_to_array_inv: Linked lists. (line 165) * gal_linkedlist_tosll_free: Linked lists. (line 416) * gal_linkedlist_tosll_into_sll: Linked lists. (line 407) * gal_mesh_change_to_full_convolution: Mesh grid for an image. (line 227) * gal_mesh_check_garray: Mesh grid for an image. (line 122) * gal_mesh_check_mesh_id: Mesh grid for an image. (line 112) * gal_mesh_ch_based_id_from_gid: Mesh grid for an image. (line 56) * gal_mesh_free_mesh: Mesh grid for an image. (line 172) * gal_mesh_full_garray: Mesh grid for an image. (line 148) * gal_mesh_gid_from_ch_based_id: Mesh grid for an image. (line 92) * gal_mesh_img_xy_to_mesh_id: Mesh grid for an image. (line 101) * gal_mesh_interpolate: Mesh grid for an image. (line 200) * gal_mesh_make_mesh: Mesh grid for an image. (line 158) * gal_mesh_operate_on_mesh: Mesh grid for an image. (line 178) * gal_mesh_smooth: Mesh grid for an image. (line 212) * gal_mesh_spatial_convolve_on_mesh: Mesh grid for an image. (line 218) * gal_mesh_value_file: Mesh grid for an image. (line 134) * gal_polygon_area: Polygons. (line 80) * gal_polygon_clip: Polygons. (line 101) * GAL_POLYGON_MAX_CORNERS: Polygons. (line 17) * gal_polygon_ordered_corners: Polygons. (line 25) * gal_polygon_pin: Polygons. (line 88) * gal_polygon_ppropin: Polygons. (line 95) * GAL_POLYGON_ROUND_ERR: Polygons. (line 20) * gal_qsort_double_decreasing: Qsort functions. (line 42) * gal_qsort_double_increasing: Qsort functions. (line 48) * gal_qsort_float_decreasing: Qsort functions. (line 30) * gal_qsort_float_increasing: Qsort functions. (line 36) * gal_qsort_index_arr: Qsort functions. (line 13) * gal_qsort_index_float_decreasing: Qsort functions. (line 54) * gal_qsort_int_decreasing: Qsort functions. (line 18) * gal_qsort_int_increasing: Qsort functions. (line 24) * gal_spatialconvolve_convolve: Spatial convolution. (line 39) * gal_spatialconvolve_params: Spatial convolution. (line 20) * gal_spatialconvolve_pparams: Spatial convolution. (line 25) * gal_spatialconvolve_thread: Spatial convolution. (line 33) * gal_statistics_cumulative_fp: Statistical operations. (line 269) * gal_statistics_double_average: Statistical operations. (line 186) * gal_statistics_double_max: Statistical operations. (line 67) * gal_statistics_double_max_return: Statistical operations. (line 73) * gal_statistics_double_min: Statistical operations. (line 54) * gal_statistics_double_min_return: Statistical operations. (line 61) * gal_statistics_d_max_with_index: Statistical operations. (line 117) * gal_statistics_d_min_max: Statistical operations. (line 103) * gal_statistics_d_min_with_index: Statistical operations. (line 124) * gal_statistics_float_average: Statistical operations. (line 180) * gal_statistics_float_max: Statistical operations. (line 48) * gal_statistics_float_max_masked: Statistical operations. (line 78) * gal_statistics_float_min: Statistical operations. (line 39) * gal_statistics_float_second_max: Statistical operations. (line 84) * gal_statistics_float_second_min: Statistical operations. (line 90) * gal_statistics_float_sum: Statistical operations. (line 134) * gal_statistics_float_sum_mask: Statistical operations. (line 151) * gal_statistics_float_sum_mask_l: Statistical operations. (line 159) * gal_statistics_float_sum_num: Statistical operations. (line 140) * gal_statistics_float_sum_squared: Statistical operations. (line 146) * gal_statistics_float_sum_squared_mask: Statistical operations. (line 166) * gal_statistics_float_sum_squared_mask_l: Statistical operations. (line 173) * gal_statistics_f_ave: Statistical operations. (line 192) * gal_statistics_f_ave_l: Statistical operations. (line 200) * gal_statistics_f_ave_std: Statistical operations. (line 207) * gal_statistics_f_ave_std_l: Statistical operations. (line 214) * gal_statistics_f_max_with_index: Statistical operations. (line 110) * gal_statistics_f_min_max: Statistical operations. (line 96) * gal_statistics_f_min_with_index: Statistical operations. (line 129) * gal_statistics_histogram: Statistical operations. (line 255) * gal_statistics_index_from_quantile: Statistical operations. (line 289) * gal_statistics_long_non_blank_max: Statistical operations. (line 32) * gal_statistics_long_non_blank_min: Statistical operations. (line 21) * GAL_STATISTICS_MAX_SIG_CLIP_CONVERGE: Statistical operations. (line 17) * gal_statistics_median: Statistical operations. (line 221) * gal_statistics_median_double_in_place: Statistical operations. (line 227) * GAL_STATISTICS_MODE_HIGH_QUANTILE: Statistical operations. (line 341) * gal_statistics_mode_index_in_sorted: Statistical operations. (line 376) * GAL_STATISTICS_MODE_LOW_QUANTILE: Statistical operations. (line 338) * GAL_STATISTICS_MODE_LOW_QUANT_GOOD: Statistical operations. (line 347) * gal_statistics_mode_mirror_plots: Statistical operations. (line 357) * gal_statistics_mode_params: Statistical operations. (line 353) * GAL_STATISTICS_MODE_SYMMETRICITY_LOW_QUANT: Statistical operations. (line 350) * GAL_STATISTICS_MODE_SYM_GOOD: Statistical operations. (line 344) * gal_statistics_mode_value_from_sym: Statistical operations. (line 367) * gal_statistics_remove_outliers_flat_cdf: Statistical operations. (line 328) * gal_statistics_save_hist: Statistical operations. (line 280) * gal_statistics_set_bins: Statistical operations. (line 235) * gal_statistics_sigma_clip_certain_num: Statistical operations. (line 311) * gal_statistics_sigma_clip_converge: Statistical operations. (line 296) * gal_threads_attr_barrier_init: Gnuastro's thread related functions. (line 19) * gal_threads_dist_in_threads: Gnuastro's thread related functions. (line 31) * GAL_THREADS_NON_THRD_INDEX: Gnuastro's thread related functions. (line 13) * gal_txtarray_array_to_txt: Text table into a C array. (line 58) * GAL_TXTARRAY_LOG: Text table into a C array. (line 14) * gal_txtarray_printf_format: Text table into a C array. (line 30) * gal_txtarray_txt_to_array: Text table into a C array. (line 20) * gal_wcs_angular_distance_deg: World Coordinate System. (line 38) * gal_wcs_pixel_area_arcsec2: World Coordinate System. (line 64) * gal_wcs_pixel_scale_deg: World Coordinate System. (line 56) * gal_wcs_radec_array_to_xy: World Coordinate System. (line 31) * gal_wcs_xy_array_to_radec: World Coordinate System. (line 14) * pthread_barrierattr_t: Implementation of pthread_barrier. (line 22) * pthread_barrier_destroy: Implementation of pthread_barrier. (line 43) * pthread_barrier_init: Implementation of pthread_barrier. (line 28) * pthread_barrier_t: Implementation of pthread_barrier. (line 25) * pthread_barrier_wait: Implementation of pthread_barrier. (line 36) Index ***** [index] * Menu: * --: Operating modes. (line 11) * --cite: Operating modes. (line 55) * --disable-guide-message: Gnuastro configure options. (line 39) * --disable-progname: Gnuastro configure options. (line 20) * --dontdelete: Input output. (line 38) * --enable-gnulibcheck: Gnuastro configure options. (line 26) * --enable-gnulibcheck <1>: Known issues. (line 34) * --enable-guide-message=no: Gnuastro configure options. (line 40) * --enable-progname: Gnuastro configure options. (line 12) * --enable-progname=no: Gnuastro configure options. (line 21) * --enable-reentrant: CFITSIO. (line 13) * --hdu: Input output. (line 10) * --help: Arguments and options. (line 12) * --help <1>: Operating modes. (line 27) * --help <2>: --help. (line 6) * --help output customization: --help. (line 55) * --keepinputdir: Input output. (line 45) * --keepinputdir <1>: Automatic output. (line 13) * --nolog: Operating modes. (line 131) * --numthreads: Operating modes. (line 136) * --numthreads <1>: Configuration files. (line 15) * --numthreads <2>: Threads in Gnuastro. (line 15) * --onlydirconf: Operating modes. (line 102) * --onlyversion: Operating modes. (line 123) * --output: Input output. (line 32) * --output <1>: Configuration files. (line 15) * --prefix: Installation directory. (line 6) * --printparams: Options. (line 66) * --printparams <1>: Operating modes. (line 72) * --printparams <2>: Final parameter values. (line 6) * --program-prefix: Executable names. (line 50) * --program-suffix: Executable names. (line 50) * --program-transform-name: Executable names. (line 50) * --quiet: Operating modes. (line 46) * --setdirconf: Operating modes. (line 77) * --setdirconf <1>: Current directory and User wide. (line 16) * --setusrconf: Operating modes. (line 98) * --setusrconf <1>: Current directory and User wide. (line 16) * --usage: Arguments and options. (line 12) * --usage <1>: Operating modes. (line 21) * --usage <2>: --usage. (line 6) * --version: Operating modes. (line 37) * --without-pgplot: WCSLIB. (line 16) * -?: Operating modes. (line 26) * -D: Input output. (line 37) * -h: Input output. (line 9) * -K: Input output. (line 44) * -mecube (ds9): Viewing multiextension FITS. (line 15) * -N: Operating modes. (line 135) * -o: Input output. (line 31) * -P: Operating modes. (line 71) * -P <1>: Final parameter values. (line 6) * -q: Operating modes. (line 45) * -S: Operating modes. (line 76) * -U: Operating modes. (line 97) * -V: Operating modes. (line 36) * ./.gnuastro/: Current directory and User wide. (line 6) * ./configure: Configuring. (line 6) * ./configure <1>: Installation directory. (line 60) * ./configure options: Gnuastro configure options. (line 6) * .bashrc: --help. (line 65) * .bashrc <1>: Generating random numbers. (line 61) * .desktop: Viewing multiextension FITS. (line 35) * 4or8: Options. (line 36) * A4 paper size: A4 print book. (line 6) * A4 print book: A4 print book. (line 6) * ACS: ImageWarp. (line 54) * Additions to Gnuastro: Suggest new feature. (line 6) * Adobe systems: Recognized file types. (line 49) * ADU: Flux Brightness and magnitude. (line 6) * ADU <1>: Instrumental noise. (line 19) * Advanced camera for surveys: ImageWarp. (line 54) * Advanced Camera for Surveys: Warping basics. (line 51) * Affine Transformation: Warping basics. (line 85) * Albert. A. Michelson: Science and its tools. (line 130) * Amplifier: Tiling an image. (line 27) * Announcements: Announcements. (line 6) * Anonymous bug submission: Report a bug. (line 84) * Anscombe F. J.: Science and its tools. (line 24) * Anscombe’s quartet: Science and its tools. (line 32) * ANSI C: Why C. (line 14) * Aperture blurring: Sigma clipping. (line 19) * Aperture photometry: Invoking astmkcatalog. (line 42) * Argp argument parser: --help. (line 55) * Argp argument parser <1>: Mandatory source code files. (line 70) * ARGP_HELP_FMT: --help. (line 55) * args.h: Mandatory source code files. (line 69) * Arguments to programs: Arguments and options. (line 6) * Array: Linked lists. (line 6) * ASCII plot: Invoking astimgstat. (line 38) * ASCII85 encoding: Invoking astconvertt. (line 101) * astprogname: Naming convention. (line 15) * Astronomical data format: Recognized file types. (line 10) * Astronomical data suffixes: Arguments. (line 20) * Astronomical Magnitude system: Flux Brightness and magnitude. (line 28) * Asynchronous thread allocation: Hubble visually checks and classifies his catalog. (line 75) * Asynchronous thread allocation <1>: Invoking astimgcrop. (line 27) * Atmosphere: Convolve. (line 25) * Atmosphere <1>: SubtractSky. (line 6) * Atmosphere blurring: Sigma clipping. (line 19) * Auto-complete in the shell: Executable names. (line 14) * Automatic configuration file writing: Configuration file format. (line 31) * Automatic output file names: Automatic output. (line 6) * Automatically created build files: Bootstrapping. (line 6) * Available number of threads: Threads in Gnuastro. (line 15) * Average filter: Grid interpolation and smoothing. (line 42) * Average, weighted: Convolve. (line 6) * AWK: Table. (line 31) * AWK <1>: Invoking astarithmetic. (line 61) * Background flux: Sky value. (line 17) * Background flux <1>: Photon counting noise. (line 45) * Background flux gradients: Photon counting noise. (line 60) * Background pixels: NoiseChisel options. (line 82) * Backup: Configure and build in RAM. (line 15) * Bash history: Final parameter values. (line 36) * Best use of CPU threads: A note on threads. (line 6) * Bi-linear interpolation: Resampling. (line 21) * Bias current: Tiling an image. (line 27) * Bias subtraction: SubtractSky. (line 6) * Bicubic interpolation: Resampling. (line 21) * Bicubic interpolation <1>: Grid interpolation and smoothing. (line 15) * Bin width, histogram: Histogram and Cumulative Frequency Plot. (line 11) * Binary image: Recognized file types. (line 72) * Binary image <1>: NoiseChisel options. (line 82) * Binary mask image values: Mask image. (line 20) * BITPIX: CFITSIO datatype. (line 15) * Black and white image: Recognized file types. (line 72) * blank color channel: Recognized file types. (line 95) * Blank pixel: Blank pixels. (line 6) * Blank pixel <1>: Arithmetic operators. (line 126) * Blank pixel <2>: Invoking astimgwarp. (line 187) * Blank pixel <3>: Invoking astsubtractsky. (line 19) * Blank pixel <4>: FITS macros and data structures. (line 24) * Blur image: Convolve. (line 25) * Blur image <1>: PSF. (line 17) * Blurring: Sigma clipping. (line 19) * Book formats: Getting help. (line 6) * Bootstrapping: Bootstrapping. (line 6) * Border on an image: Invoking astconvertt. (line 80) * Breadth first search: Defining an ellipse. (line 31) * Brightness: Galaxies. (line 11) * Brightness <1>: Flux Brightness and magnitude. (line 13) * Brightness <2>: Profile magnitude. (line 6) * Buffers (Emacs): Coding conventions. (line 44) * Bug: Report a bug. (line 6) * Bug <1>: Gnuastro project webpage. (line 6) * Bug reporting: Report a bug. (line 16) * Bug tracker: Report a bug. (line 97) * bug-gnuastro@gnu.org: Report a bug. (line 78) * Build: Quick start. (line 6) * Build individual profiles: MakeProfiles options. (line 83) * Build tree: Test scripts. (line 23) * Building from source: Mandatory dependencies. (line 13) * C programming language: Why C. (line 6) * C++ programming language: Why C. (line 6) * C, plotting: PGPLOT. (line 6) * Cache, system: A note on threads. (line 29) * Camera: Resampling. (line 6) * CANDELS: Quantifying data limits. (line 56) * CCD: ImageWarp. (line 54) * CCD <1>: Tiling an image. (line 27) * Central management: Gnuastro project webpage. (line 6) * CFITSIO: CFITSIO. (line 6) * CFITSIO <1>: FITS files. (line 6) * CFITSIO <2>: CFITSIO datatype. (line 15) * CFITSIO version on outputs: Output headers. (line 6) * Change converted pixel values: Invoking astconvertt. (line 130) * Channel: Tiling an image. (line 37) * Charge-coupled device: ImageWarp. (line 54) * Check: Quick start. (line 6) * Check center of crop: astimgcrop options. (line 166) * Checking detection algorithms: MakeProfiles. (line 6) * Checking final parameter values: Final parameter values. (line 6) * Checking tests: Tests. (line 6) * Citation information: Mandatory source code files. (line 126) * cite.h: Mandatory source code files. (line 125) * CLI: command-line user interface: Command-line interface. (line 6) * CLI: repeating operations: Command-line interface. (line 52) * Clump magnitude limit: Quantifying data limits. (line 6) * CMYK: Color. (line 6) * Colorspace: Color. (line 6) * Colorspace, grayscale: Color. (line 6) * Colorspace, transformation: Color. (line 28) * Command-line arguments: Arguments and options. (line 6) * Command-line help: Getting help. (line 13) * Command-line options: Arguments and options. (line 6) * Command-line scroll: --help. (line 27) * Command-line searching text: --help. (line 47) * Command-line token separation: Command-line. (line 11) * Command-line user interface: Command-line interface. (line 6) * Command-line, long outputs: --help. (line 22) * Command-line, viewing full book: Info. (line 6) * Commutative property: Merging multiple warpings. (line 6) * Comoving distance: Distance on a 2D curved space. (line 154) * Compare Moffat and Gaussian: PSF. (line 66) * Compare Poisson and Gaussian: Photon counting noise. (line 32) * Compile: Quick start. (line 6) * Compiled PostScript: Recognized file types. (line 49) * Compiling from source: Mandatory dependencies. (line 13) * Completeness: Quantifying data limits. (line 119) * Complex numbers: Invoking astconvolve. (line 69) * Compression quality in JPEG: Invoking astconvertt. (line 117) * Configuration file directories: Configuration file precedence. (line 6) * Configuration file format: Configuration file format. (line 11) * Configuration file precedence: Configuration file precedence. (line 6) * Configuration file suffix: Configuration file format. (line 6) * Configuration files: Options. (line 86) * Configuration files <1>: Configuration files. (line 6) * Configuration files, system wide: System wide. (line 6) * Configuration files, writing: Configuration file format. (line 31) * Configuration, not finding library: Known issues. (line 11) * Configure options: Configuring. (line 12) * Configure options particular to Gnuastro: Gnuastro configure options. (line 6) * Configuring: Configuring. (line 6) * Convenient book formats: Getting help. (line 6) * Convention for program source: Program source. (line 6) * Converting data formats: ConvertType. (line 6) * Converting image formats: ConvertType. (line 6) * ConvertType (astconvertt): ConvertType. (line 6) * Convex Hull: Polygons. (line 57) * Convolution: Convolve. (line 6) * Convolution <1>: Convolution process. (line 24) * Convolution <2>: PSF. (line 17) * Convolution kernel: FITS functions. (line 336) * Cookbook: Tutorials. (line 6) * Coordinate transformation: Warping basics. (line 6) * Coordinates, homogeneous: Warping basics. (line 63) * Copyright: Your rights. (line 12) * Correlated noise: Quantifying data limits. (line 105) * Correlation: Convolution process. (line 24) * Cosmic ray removal: Sky value. (line 23) * Cosmic rays: Convolve. (line 25) * Cosmic rays <1>: ImageWarp. (line 37) * Cosmic rays <2>: Sky value. (line 16) * Cosmic rays <3>: Finding the sky value. (line 18) * Cosmic rays <4>: Sigma clipping. (line 19) * COSMOS survey: ImageCrop. (line 13) * Counting error: Photon counting noise. (line 6) * Counting from zero.: Options. (line 106) * Counts: Flux Brightness and magnitude. (line 6) * Counts <1>: Instrumental noise. (line 19) * CPPFLAGS: Known issues. (line 46) * CPPFLAGS <1>: Headers. (line 153) * CPU threads: Threads in Gnuastro. (line 6) * CPU threads <1>: MakeProfiles options. (line 199) * CPU threads, number: Configuration files. (line 15) * CPU threads, set number: Operating modes. (line 135) * CPU, using all threads: Threads in Gnuastro. (line 6) * Crop a given section of image: Crop section syntax. (line 6) * Crop part of image: ImageCrop. (line 6) * Crop section format: Crop section syntax. (line 25) * Cumulative Frequency Plot: Histogram and Cumulative Frequency Plot. (line 20) * Customize --help output: --help. (line 55) * Customize executable names: Executable names. (line 28) * Customizing installation: Configuring. (line 12) * Data: Finding the sky value. (line 6) * Data format conversion: ConvertType. (line 6) * Data structures: Headers. (line 89) * Data type: CFITSIO datatype. (line 6) * de Vaucouleur profile: Galaxies. (line 11) * Debugging: Building and debugging. (line 35) * Default executable search directory: Installation directory. (line 60) * Default library search directory: Installation directory. (line 149) * Default option values: Options. (line 86) * Default option values <1>: Configuration files. (line 6) * Define section to crop: Crop section syntax. (line 12) * Dependencies, Gnuastro: Mandatory dependencies. (line 6) * Depth: Quantifying data limits. (line 6) * Depth <1>: Quantifying data limits. (line 41) * Detached threads: Gnuastro's thread related functions. (line 23) * Detection: Convolve. (line 25) * Detection <1>: NoiseChisel. (line 26) * Detections false: Quantifying data limits. (line 131) * Detector: Resampling. (line 6) * Development packages: Known issues. (line 11) * Diffraction limited: PSF. (line 6) * Directory, install: Installation directory. (line 134) * Discrete Fourier transform: Invoking astconvolve. (line 44) * Distortion, optical: ImageWarp. (line 48) * Distribution mean: Finding the sky value. (line 6) * Distribution median: Finding the sky value. (line 6) * Distribution mode: Finding the sky value. (line 6) * Distribution mode <1>: Sky value misconceptions. (line 20) * Douglas Rushkoff: Science and its tools. (line 46) * Drizzle: Resampling. (line 48) * Dynamic linking: Linking. (line 55) * Edges, image: Resampling. (line 32) * Edwin Hubble: Hubble visually checks and classifies his catalog. (line 6) * Effective radius: Galaxies. (line 11) * Efficient use of CPU threads: A note on threads. (line 6) * Ellipse: Defining an ellipse. (line 6) * Elliptical distance: Defining an ellipse. (line 26) * Elliptical galaxies: Hubble visually checks and classifies his catalog. (line 115) * Emacs buffers: Coding conventions. (line 44) * Encapsulated PostScript: Recognized file types. (line 41) * Environment: Installation directory. (line 40) * Environment variable, HOME: Installation directory. (line 53) * Environment variables: Installation directory. (line 33) * Environment variables <1>: Installation directory. (line 40) * Environment variables <2>: Generating random numbers. (line 26) * eog: Hubble visually checks and classifies his catalog. (line 102) * EPS: Recognized file types. (line 41) * Erosion: NoiseChisel options. (line 99) * Error, floating point round-off: Invoking astconvolve. (line 83) * etc: Configuration files. (line 6) * Exact area resampling: Resampling. (line 48) * Executable names: Executable names. (line 6) * Eye of GNOME: Hubble visually checks and classifies his catalog. (line 102) * False detections: Quantifying data limits. (line 131) * Feature request: Gnuastro project webpage. (line 6) * Feature requests: Suggest new feature. (line 6) * File I/O: Configure and build in RAM. (line 6) * File operations: Extensions and Tables. (line 6) * File suffix mis-spelling: Recognized file types. (line 108) * File system Hierarchy Standard: Configuration files. (line 6) * file systems, tmpfs: Configure and build in RAM. (line 23) * Final parameter value checking: Final parameter values. (line 6) * first-in-first-out: FITS macros and data structures. (line 76) * first-in-first-out <1>: FITS functions. (line 146) * first-in-first-out <2>: Linked lists. (line 32) * FITS: FITS files. (line 6) * FITS image viewer: SAO ds9. (line 6) * FITS standard: CFITSIO. (line 6) * FITS standard <1>: Invoking astimgwarp. (line 51) * FITS: data type: CFITSIO datatype. (line 6) * Fitting: Modeling and fittings. (line 6) * Flat field: SubtractSky. (line 6) * Flip coordinates: Warping basics. (line 30) * Floating point error: Measuring elliptical parameters. (line 50) * Floating point round-off error: Invoking astconvolve. (line 83) * FLT: Options. (line 40) * Flux: Flux Brightness and magnitude. (line 13) * Flux to magnitude conversion: Flux Brightness and magnitude. (line 28) * Foreground pixels: NoiseChisel options. (line 82) * Fourier spectrum: Invoking astconvolve. (line 69) * Free software: Your rights. (line 12) * Free Software Foundation: Contributing to Gnuastro. (line 16) * FSF: Contributing to Gnuastro. (line 16) * Full Width at Half Maximum: PSF. (line 27) * Function gradient over pixel area: Sampling from a function. (line 16) * Function groups: Coding conventions. (line 158) * Functions for user interface: Mandatory source code files. (line 79) * FWHM: PSF. (line 27) * Gain: Flux Brightness and magnitude. (line 6) * Gain <1>: Instrumental noise. (line 19) * Galaxy profiles: Galaxies. (line 6) * Galileo, G.: Science and its tools. (line 100) * Gaussian: Invoking astnoisechisel. (line 17) * Gaussian <1>: Invoking astmkcatalog. (line 20) * Gaussian distribution: Quantifying signal in a mesh. (line 6) * Gaussian distribution <1>: PSF. (line 37) * Gaussian FWHM: PSF. (line 50) * GCC: Summary and example on libraries. (line 30) * Gedit: Hubble visually checks and classifies his catalog. (line 145) * Gedit <1>: Sufi simulates a detection. (line 288) * General file operations: Extensions and Tables. (line 6) * Generalized de Vaucouleur profile: Galaxies. (line 6) * Git: Optional dependencies. (line 23) * Git <1>: Version controlled source. (line 6) * Git <2>: Git wrappers. (line 6) * GNOME 2: Viewing multiextension FITS. (line 58) * GNOME 3: Command-line interface. (line 18) * GNOME 3 <1>: Viewing multiextension FITS. (line 30) * GNU Astronomy Utilities (Gnuastro): Introduction. (line 6) * GNU Autoconf: Bootstrapping dependencies. (line 61) * GNU Autoconf <1>: Bootstrapping. (line 60) * GNU Autoconf <2>: Synchronizing. (line 21) * GNU Autoconf <3>: Configuring. (line 21) * GNU Autoconf <4>: Building and debugging. (line 6) * GNU Autoconf Archive: Bootstrapping dependencies. (line 65) * GNU Autoconf Archive <1>: Bootstrapping. (line 6) * GNU Automake: Bootstrapping dependencies. (line 55) * GNU Automake <1>: Bootstrapping. (line 60) * GNU Automake <2>: Building and debugging. (line 6) * GNU AWK: Table. (line 31) * GNU AWK <1>: Invoking astarithmetic. (line 61) * GNU Bash: Command-line interface. (line 52) * GNU Bash <1>: Hubble visually checks and classifies his catalog. (line 115) * GNU Bash <2>: Installation directory. (line 97) * GNU Bash <3>: Installation directory. (line 106) * GNU Bash <4>: Invoking astheader. (line 87) * GNU Bash <5>: Program design philosophy. (line 26) * GNU Binutils: Linking. (line 16) * GNU build system: Mandatory dependencies. (line 6) * GNU build system <1>: Bootstrapping. (line 60) * GNU build system <2>: Installation directory. (line 134) * GNU build system <3>: Configure and build in RAM. (line 34) * GNU build system <4>: Headers. (line 153) * GNU build system <5>: Headers. (line 162) * GNU build system <6>: Building and debugging. (line 6) * GNU C library: New to GNU/Linux?. (line 19) * GNU C library <1>: Bootstrapping dependencies. (line 28) * GNU C library <2>: Bootstrapping. (line 60) * GNU C library <3>: Gnuastro configure options. (line 27) * GNU C library <4>: Configure and build in RAM. (line 34) * GNU C library <5>: Info. (line 28) * GNU C library <6>: Adding new columns to MakeCatalog. (line 47) * GNU C library <7>: Linking. (line 101) * GNU C library <8>: Coding conventions. (line 91) * GNU coding standards: Introduction. (line 6) * GNU coding standards <1>: Coding conventions. (line 6) * GNU coding standards <2>: Coding conventions. (line 134) * GNU Compiler Collection: New to GNU/Linux?. (line 19) * GNU Compiler Collection <1>: Summary and example on libraries. (line 30) * GNU Compiler Collection <2>: Coding conventions. (line 37) * GNU Coreutils: Threads in Gnuastro. (line 6) * GNU Coreutils <1>: Program design philosophy. (line 18) * GNU Emacs: Command-line interface. (line 75) * GNU Emacs <1>: Hubble visually checks and classifies his catalog. (line 115) * GNU Emacs <2>: Hubble visually checks and classifies his catalog. (line 145) * GNU Emacs <3>: Sufi simulates a detection. (line 288) * GNU Emacs <4>: Configure and build in RAM. (line 50) * GNU Emacs <5>: Info. (line 28) * GNU Emacs <6>: Coding conventions. (line 151) * GNU Emacs <7>: Coding conventions. (line 158) * GNU Emacs <8>: Coding conventions. (line 188) * GNU Free Documentation License: Your rights. (line 40) * GNU Free Documentation License <1>: GNU Free Documentation License. (line 6) * GNU General Public License: Your rights. (line 40) * GNU Grep: --help. (line 47) * GNU Grep <1>: Invoking astheader. (line 60) * GNU Grep <2>: Invoking astcosmiccal. (line 36) * GNU help2man: Bootstrapping dependencies. (line 77) * GNU Info: Info. (line 6) * GNU Libtool: Bootstrapping dependencies. (line 71) * GNU Libtool <1>: Bootstrapping. (line 60) * GNU Libtool <2>: Known issues. (line 88) * GNU Libtool <3>: Linking. (line 6) * GNU Libtool <4>: Linking. (line 55) * GNU Libtool <5>: Linking. (line 130) * GNU Libtool <6>: Automatic linking script. (line 18) * GNU Libtool <7>: Building and debugging. (line 6) * GNU Parallel: Hubble visually checks and classifies his catalog. (line 89) * GNU Parallel <1>: How to run simultaneous operations. (line 15) * GNU portability library: Known issues. (line 52) * GNU Portability Library (Gnulib): Bootstrapping dependencies. (line 28) * GNU Portability Library (Gnulib) <1>: Bootstrapping. (line 6) * GNU Portability Library (Gnulib) <2>: Gnuastro configure options. (line 27) * GNU Portability Library (Gnulib) <3>: Known issues. (line 34) * GNU Portability Library (Gnulib) <4>: Coding conventions. (line 86) * GNU Scientific Library: GNU Scientific Library. (line 6) * GNU Scientific Library <1>: Generating random numbers. (line 26) * GNU software documentation: Info. (line 22) * GNU style options: Options. (line 6) * GNU Tar: Quick start. (line 6) * GNU Texinfo: Your rights. (line 6) * GNU Texinfo <1>: Bootstrapping. (line 60) * GNU Texinfo <2>: A4 print book. (line 13) * GNU Texinfo <3>: Known issues. (line 83) * GNU/Linux: New to GNU/Linux?. (line 19) * Gnuastro coding convention: Coding conventions. (line 6) * Gnuastro common options: Common options. (line 6) * Gnuastro major version number: GNU Astronomy Utilities 1.0. (line 6) * Gnuastro program structure convention: Program source. (line 6) * Gnuastro project page: Report a bug. (line 84) * Gnuastro test scripts: Test scripts. (line 6) * Gnulib: GNU Portability Library: Bootstrapping dependencies. (line 28) * Gnulib: GNU Portability Library <1>: Bootstrapping. (line 6) * Gnulib: GNU Portability Library <2>: Gnuastro configure options. (line 27) * Gnulib: GNU Portability Library <3>: Known issues. (line 34) * Gnulib: GNU Portability Library <4>: Coding conventions. (line 86) * GPL Ghostscript: Optional dependencies. (line 10) * GPL Ghostscript <1>: Optional dependencies. (line 41) * GPL Ghostscript <2>: Known issues. (line 74) * GPL Ghostscript <3>: Recognized file types. (line 86) * Gradient: SubtractSky. (line 17) * Gradient <1>: Tiling an image. (line 6) * Gradient over pixel area: Sampling from a function. (line 16) * Gradients in background flux: Photon counting noise. (line 60) * Graphic user interface: Command-line interface. (line 6) * Gravitational lensing: ImageWarp. (line 13) * Grayscale: Color. (line 6) * Grid: SubtractSky. (line 17) * Grid <1>: Tiling an image. (line 6) * Groups of similar functions: Coding conventions. (line 158) * GUI: graphic user interface: Command-line interface. (line 6) * GUI: repeating operations: Command-line interface. (line 43) * Gzip: Release tarball. (line 37) * Gérard de Vaucouleurs: Galaxies. (line 11) * Halted program: Report a bug. (line 6) * HDD: Configure and build in RAM. (line 12) * HDU: Arguments and options. (line 26) * HDU <1>: Input output. (line 9) * HDU <2>: Invoking astheader. (line 19) * Header data unit: Arguments and options. (line 26) * Header data unit <1>: Input output. (line 9) * Header file: Coding conventions. (line 70) * Help: Getting help. (line 6) * help-gnuastro mailing list: help-gnuastro mailing list. (line 6) * help-gnuastro@gnu.org: help-gnuastro mailing list. (line 13) * Hexadecimal encoding: Invoking astconvertt. (line 101) * Histogram: Sky value misconceptions. (line 20) * Histogram <1>: Histogram and Cumulative Frequency Plot. (line 11) * HOME: Installation directory. (line 53) * HOME <1>: Current directory and User wide. (line 6) * HOME/.local/: Installation directory. (line 53) * HOME/.local/etc/: Current directory and User wide. (line 6) * Homogeneous coordinates: Warping basics. (line 63) * Homography: Warping basics. (line 93) * Hubble Space Telescope: ImageCrop. (line 13) * Hubble Space Telescope <1>: ImageWarp. (line 54) * Hubble Space Telescope <2>: Warping basics. (line 51) * Hubble Space Telescope <3>: Tiling an image. (line 27) * Hyper Suprime-Cam: Tiling an image. (line 27) * IEEE NaN: FITS macros and data structures. (line 33) * IEEE NaN <1>: Mesh grid for an image. (line 183) * IEEE NaN <2>: Mesh grid for an image. (line 204) * Image: Color. (line 6) * Image blurring: PSF. (line 17) * Image edges: Resampling. (line 32) * Image format conversion: ConvertType. (line 6) * Image mosaic: ImageCrop. (line 13) * Image mosaic <1>: ImageWarp. (line 30) * Image noise: Noise basics. (line 6) * Image tiles: ImageCrop. (line 13) * Image transformations: MakeProfiles. (line 41) * ImageCrop (astimgcrop): ImageCrop. (line 6) * ImageMagick: Bootstrapping dependencies. (line 113) * Imaging surveys: ImageCrop. (line 13) * Inconsistent results: Report a bug. (line 6) * Individual profiles: MakeProfiles options. (line 83) * info-gnuastro@gnu.org: Synchronizing. (line 21) * INFOPATH: Installation directory. (line 149) * Input/Output, file: Configure and build in RAM. (line 6) * Inside-out construction: Defining an ellipse. (line 31) * Inside-out construction <1>: Sampling from a function. (line 43) * Install directory: Installation directory. (line 134) * Install with no super-user access: Installation directory. (line 6) * Installation: Installation. (line 6) * Installation, customizing: Configuring. (line 12) * Installed help methods: Getting help. (line 22) * Instrumental noise: Instrumental noise. (line 6) * INT: Options. (line 30) * Integration over pixel: Sampling from a function. (line 16) * Integration to infinity: Profile magnitude. (line 15) * Internal default value: Configuration files. (line 15) * Internally stored option value: Threads in Gnuastro. (line 15) * Interpolation: Resampling. (line 21) * Interpolation, bi-linear: Resampling. (line 21) * Interpolation, bi-linear <1>: Grid interpolation and smoothing. (line 15) * Interpolation, bicubic: Resampling. (line 21) * Interpolation, bicubic <1>: Grid interpolation and smoothing. (line 15) * Interpolation, spline: Grid interpolation and smoothing. (line 15) * Intervals, histogram: Histogram and Cumulative Frequency Plot. (line 11) * Irrelevant options: Common options. (line 13) * isnan: FITS macros and data structures. (line 33) * ISO C90: Why C. (line 14) * Issue: Gnuastro project webpage. (line 6) * Jaynes E. T.: Science and its tools. (line 148) * JPEG compression quality: Invoking astconvertt. (line 117) * JPEG format: Optional dependencies. (line 30) * JPEG format <1>: Recognized file types. (line 23) * Ken Thomson: Science and its tools. (line 111) * Kernel, convolution: Convolve. (line 6) * Kernel: convolution: FITS functions. (line 336) * Kernighan, Brian: Why C. (line 14) * Labeled image: FITS functions. (line 327) * Large astronomical images: ImageCrop. (line 6) * last-in-first-out: FITS macros and data structures. (line 76) * last-in-first-out <1>: FITS functions. (line 136) * last-in-first-out <2>: Linked lists. (line 32) * LaTeX: Bootstrapping dependencies. (line 81) * LaTeX <1>: Recognized file types. (line 60) * Lawrence Livermore National Laboratory: Multithreaded programming. (line 20) * LDFLAGS: Known issues. (line 24) * LD_LIBRARY_PATH: Installation directory. (line 149) * LD_LIBRARY_PATH <1>: Known issues. (line 64) * LD_LIBRARY_PATH <2>: PGPLOT. (line 62) * Learning GNU Info: Info. (line 22) * Lensing simulations: MakeProfiles. (line 41) * less: --help. (line 33) * libgit2: Optional dependencies. (line 23) * libgit2 <1>: Git wrappers. (line 6) * libjpeg: Optional dependencies. (line 30) * Library search directory: Installation directory. (line 149) * Library: shared: Linking. (line 55) * Limit, object/clump magnitude: Quantifying data limits. (line 6) * Linear interpolation: Grid interpolation and smoothing. (line 15) * Linear spatial filtering: Convolution process. (line 16) * Linked list: FITS macros and data structures. (line 76) * Linked list <1>: Linked lists. (line 6) * Linking: dynamic: Linking. (line 55) * Linking: Static: Linking. (line 31) * Linux: New to GNU/Linux?. (line 19) * Linux kernel: Configure and build in RAM. (line 34) * Long option abbreviation: Options. (line 66) * Long outputs: --help. (line 22) * Lord Kelvin: Science and its tools. (line 124) * Low level programming: Why C. (line 82) * Luminosity: Flux Brightness and magnitude. (line 13) * Lzip: Release tarball. (line 37) * Macro: Headers. (line 89) * Magnitude zero-point: Flux Brightness and magnitude. (line 28) * Magnitude, object/clump detection limit: Quantifying data limits. (line 6) * Magnitude, upper limit: Quantifying data limits. (line 91) * Magnitudes from flux: Flux Brightness and magnitude. (line 28) * Mailing list archives: Report a bug. (line 78) * Mailing list archives <1>: help-gnuastro mailing list. (line 13) * Mailing list: bug-gnuastro: Report a bug. (line 78) * Mailing list: bug-gnuastro <1>: Gnuastro project webpage. (line 18) * Mailing list: gnuastro-commits: Developing mailing lists. (line 37) * Mailing list: gnuastro-commits <1>: Commit guidelines. (line 34) * Mailing list: gnuastro-commits <2>: Commit guidelines. (line 50) * Mailing list: gnuastro-commits <3>: Commit guidelines. (line 72) * Mailing list: gnuastro-devel: Gnuastro project webpage. (line 57) * Mailing list: gnuastro-devel <1>: Developing mailing lists. (line 13) * Mailing list: help-gnuastro: help-gnuastro mailing list. (line 6) * Mailing list: info-gnuastro: Version numbering. (line 6) * Mailing list: info-gnuastro <1>: Announcements. (line 6) * Mailing list: info-gnuastro <2>: Synchronizing. (line 21) * main function: Mandatory source code files. (line 15) * Main parameters C structure: Mandatory source code files. (line 26) * main.c: Mandatory source code files. (line 14) * main.h: Mandatory source code files. (line 25) * Major version number: Version numbering. (line 6) * make check: Tests. (line 6) * MakeProfiles (astmkprof): MakeProfiles. (line 6) * Making a distribution package: Developer's checklist. (line 24) * Making profiles pixel by pixel: Defining an ellipse. (line 31) * Man pages: Man pages. (line 6) * Management hub: Gnuastro project webpage. (line 6) * Mandatory arguments: Arguments and options. (line 12) * Mandatory arguments <1>: --usage. (line 6) * MANPATH: Installation directory. (line 149) * Mask image: Invoking astarithmetic. (line 32) * Mask image <1>: Mask image. (line 6) * Matplotlib: Mirror distribution. (line 58) * Matplotlib, Python: Program design philosophy. (line 26) * Matplotlib, Python <1>: PGPLOT. (line 14) * Matrix: Warping basics. (line 17) * Matrix multiplication: Merging multiple warpings. (line 6) * Mean of distribution: Finding the sky value. (line 6) * Median of distribution: Finding the sky value. (line 6) * Mesh: SubtractSky. (line 17) * Mesh grid: Tiling an image. (line 6) * Metacharacters: Command-line. (line 11) * Metacharacters on the command-line: Arguments and options. (line 19) * Michelson, Albert. A.: Science and its tools. (line 130) * Minor version number: Version numbering. (line 6) * Mirror distribution: Mirror distribution. (line 6) * Mis-spelling file suffix: Recognized file types. (line 108) * Mixing pixel values: Convolve. (line 25) * Mixing pixel values <1>: Resampling. (line 6) * mock.fits: Tests. (line 6) * Mode of a distribution: Sky value misconceptions. (line 20) * Mode of distribution: Finding the sky value. (line 6) * Modeling: Modeling and fittings. (line 6) * Modeling stars: Stars. (line 6) * Modifying print book: A4 print book. (line 6) * Modularity: Review of library fundamentals. (line 18) * Moffat beta: PSF. (line 59) * Moffat function: PSF. (line 53) * Moffat FWHM: PSF. (line 64) * Moments: Measuring elliptical parameters. (line 19) * Monte carlo integration: Sampling from a function. (line 26) * Mosaicing: ImageCrop. (line 13) * Mosaicing <1>: ImageWarp. (line 30) * Multi-threaded programs: Threads in Gnuastro. (line 6) * Multiextention FITS: Viewing multiextension FITS. (line 6) * Multiple file opening, reentrancy: CFITSIO. (line 13) * Multiplication, Matrix: Warping basics. (line 17) * Multiplication, matrix: Merging multiple warpings. (line 6) * Multithreaded programming: Multithreaded programming. (line 6) * Möbius, August. F.: Warping basics. (line 63) * Names of executables: Executable names. (line 6) * Names, customize: Executable names. (line 28) * Names, programs: Naming convention. (line 6) * NaN: Arithmetic operators. (line 60) * NaN <1>: Invoking astarithmetic. (line 32) * NaN <2>: Invoking astimgwarp. (line 155) * NaN <3>: Mask image. (line 36) * NaN <4>: Invoking astimgstat. (line 120) * NaN <5>: NoiseChisel options. (line 92) * NaN <6>: Invoking astmkcatalog. (line 144) * NaN <7>: Array manipulation. (line 74) * NaN <8>: FITS macros and data structures. (line 33) * NaN <9>: Mesh grid for an image. (line 183) * NaN <10>: Mesh grid for an image. (line 204) * Navigating source files: Program source. (line 6) * Necessary parameters: Configuration files. (line 6) * Neighborhood: Convolve. (line 6) * No access to super-user install: Installation directory. (line 6) * Noise: Quantifying signal in a mesh. (line 6) * Noise <1>: MakeNoise. (line 6) * Noise <2>: Noise basics. (line 6) * Noise simulation: Photon counting noise. (line 66) * Noise, instrumental: Instrumental noise. (line 6) * Noise-based detection: NoiseChisel. (line 34) * Non-commutative operations: Merging multiple warpings. (line 6) * Normalizing histogram: Histogram and Cumulative Frequency Plot. (line 11) * nproc: Threads in Gnuastro. (line 6) * Number of CPU threads to use: Operating modes. (line 135) * Number of CPU threads to use <1>: Configuration files. (line 15) * Number of threads available: Threads in Gnuastro. (line 15) * Number, version: Version numbering. (line 6) * Numbers, complex: Invoking astconvolve. (line 69) * Numbers, psudo-random: Generating random numbers. (line 14) * Numbers, random: Generating random numbers. (line 6) * Object magnitude limit: Quantifying data limits. (line 6) * Object oriented programming: Why C. (line 26) * On/Off options: Options. (line 23) * Online help: Getting help. (line 13) * Opening multiextention FITS: Viewing multiextension FITS. (line 6) * OpenMP: Multithreaded programming. (line 31) * Operations on files: Extensions and Tables. (line 6) * Operations, non-commutative: Merging multiple warpings. (line 6) * Operator, structure de-reference: Mandatory source code files. (line 57) * Optical distortion: ImageWarp. (line 48) * Optimization: Building and debugging. (line 35) * Optimization flag: Coding conventions. (line 37) * Option values: Options. (line 49) * Optional and mandatory tokens: --usage. (line 6) * Options: Invoking astarithmetic. (line 47) * Options common to all programs: Common options. (line 6) * Options to programs: Arguments and options. (line 6) * Options, abbreviation: Options. (line 66) * Options, GNU style: Options. (line 6) * Options, irrelevant: Common options. (line 13) * Options, on/off: Options. (line 23) * Options, repeated: Options. (line 74) * Options, short (-) and long (--): Options. (line 6) * Order in search directory: Installation directory. (line 182) * Output file names, automatic: Automatic output. (line 6) * Output FITS headers: Output headers. (line 6) * Output, wrong: Report a bug. (line 6) * Oversample: Sufi simulates a detection. (line 160) * Oversampling: Oversampling. (line 6) * p: Mandatory source code files. (line 51) * Package managers: Mandatory dependencies. (line 13) * Paper size, A4: A4 print book. (line 6) * Paper size, US letter: A4 print book. (line 6) * Parametric PSFs: PSF. (line 27) * PATH: Installation directory. (line 60) * PDF: Recognized file types. (line 49) * PGFplots in TeX or LaTeX: Program design philosophy. (line 26) * PGFplots in TeX or LaTeX <1>: PGPLOT. (line 14) * PGPLOT: PGPLOT. (line 6) * Phase angle: Invoking astconvolve. (line 69) * photo-electrons: Sky value. (line 46) * Photoelectrons: Resampling. (line 6) * Photometry, aperture: Invoking astmkcatalog. (line 42) * Photon counting noise: Photon counting noise. (line 6) * Picture element: Resampling. (line 6) * Pipe: --help. (line 33) * Pixel: Resampling. (line 6) * Pixel by pixel making of profiles: Defining an ellipse. (line 31) * Pixel mixing: Convolve. (line 25) * Pixel mixing <1>: Resampling. (line 6) * Pixel mixing <2>: Resampling. (line 48) * Pixel, blank: Invoking astimgwarp. (line 187) * Pixelated graphics: Recognized file types. (line 23) * Pixels: Color. (line 6) * Plain text: Recognized file types. (line 100) * Plotting directly in C: PGPLOT. (line 6) * PNG: Mirror distribution. (line 58) * PNG standard: Color. (line 40) * Point pixels: Resampling. (line 21) * Point source: PSF. (line 6) * Point Spread Function: PSF. (line 6) * Poisson distribution: Photon counting noise. (line 22) * Portable Document format: Recognized file types. (line 49) * Position angle: Measuring elliptical parameters. (line 128) * POSIX threads: Implementation of pthread_barrier. (line 6) * POSIX threads library: Threads in Gnuastro. (line 6) * POSIX threads library <1>: Multithreaded programming. (line 20) * Postage stamp images: ImageCrop. (line 6) * Postfix notation: Reverse polish notation. (line 6) * PostScript: Recognized file types. (line 41) * PostScript vs. PDF: Recognized file types. (line 49) * Pre-Processor: Headers. (line 6) * Pre-processor macros: Headers. (line 89) * Precedence, configuration files: Configuration file precedence. (line 6) * prefix/etc/: System wide. (line 6) * Primary colors: Color. (line 6) * Probability density function: Sky value misconceptions. (line 20) * Probability distribution function: Histogram and Cumulative Frequency Plot. (line 11) * Profiles, galaxies: Galaxies. (line 6) * progname.c: Mandatory source code files. (line 101) * prognameparams: Mandatory source code files. (line 26) * Program crashing: Report a bug. (line 6) * Program names: Naming convention. (line 6) * Program structure convention: Program source. (line 6) * Programming, low level: Why C. (line 82) * ProgramName: Naming convention. (line 15) * Projective transformation: Warping basics. (line 93) * Proper distance: Distance on a 2D curved space. (line 124) * PSF: Grid interpolation and smoothing. (line 31) * PSF <1>: PSF. (line 6) * PSF image size: PSF. (line 17) * PSF over-sample: Oversampling. (line 12) * PSF width: PSF. (line 27) * PSF, Moffat compared Gaussian: PSF. (line 66) * Psudo-random numbers: Generating random numbers. (line 14) * pthread: Threads in Gnuastro. (line 6) * Pthread: Mesh grid for an image. (line 183) * pthread_barrier: Implementation of pthread_barrier. (line 6) * Public domain: Your rights. (line 12) * Purity: Quantifying data limits. (line 131) * Puzzle solving scientist: Science and its tools. (line 137) * Python: Mirror distribution. (line 23) * Python Matplotlib: Program design philosophy. (line 26) * Python Matplotlib <1>: PGPLOT. (line 14) * Python programming language: Why C. (line 6) * Quality of compression in JPEG: Invoking astconvertt. (line 117) * Quantile: NoiseChisel options. (line 82) * Radial profile on ellipse: Defining an ellipse. (line 15) * Radius, effective: Galaxies. (line 11) * Random numbers: Generating random numbers. (line 6) * Raster graphics: Recognized file types. (line 23) * Readout noise: Instrumental noise. (line 6) * Redirection of output: Final parameter values. (line 36) * Redirection of output <1>: --help. (line 22) * Redirection of output <2>: --help. (line 42) * Reentrancy, multiple file opening: CFITSIO. (line 13) * Remembering options: Getting help. (line 6) * Remote operation: Command-line interface. (line 91) * Removing ast from executables: Executable names. (line 70) * Repeated options: Options. (line 74) * Report a bug: Gnuastro project webpage. (line 6) * Reproducibility: Invoking astmkcatalog. (line 212) * Reproducible bug reports: Report a bug. (line 64) * Reproducible results: Command-line interface. (line 52) * Reproducible results <1>: Final parameter values. (line 46) * Resampling: Resampling. (line 6) * Resource heavy operations: Command-line interface. (line 83) * Results, wrong: Report a bug. (line 6) * Reverse Polish Notation: Reverse polish notation. (line 6) * RGB: Color. (line 6) * Ritchie, Dennis: Why C. (line 14) * Root access, not possible: Installation directory. (line 6) * Root parameter structure: Mandatory source code files. (line 26) * Rotation of coordinates: Warping basics. (line 17) * Round-off error: Invoking astconvolve. (line 83) * Round-off error <1>: Polygons. (line 21) * rpl_malloc: Known issues. (line 52) * Sampling: Resampling. (line 6) * Sampling <1>: Sampling from a function. (line 6) * SAO ds9: SAO ds9. (line 6) * Save output to file: --help. (line 42) * Saving binary image: Recognized file types. (line 72) * Scaling: Warping basics. (line 6) * Scientist, puzzle solver: Science and its tools. (line 137) * Scripts, startup: Installation directory. (line 97) * Scroll command-line: --help. (line 27) * Search directory for executables: Installation directory. (line 60) * Search directory order: Installation directory. (line 182) * Searching text: --help. (line 47) * Second moment: Measuring elliptical parameters. (line 28) * Section of an image: ImageCrop. (line 6) * Secure shell: Command-line interface. (line 91) * SED, stream editor: Executable names. (line 60) * Seed, psudo-random numbers: Generating random numbers. (line 14) * Segmentation map: FITS functions. (line 327) * Separating tokens on the command-line: Command-line. (line 11) * setparams function: Mandatory source code files. (line 90) * Setting output file names automatically: Automatic output. (line 6) * Setting PATH: Installation directory. (line 60) * Shared library: Linking. (line 55) * Shared library versioning: Linking. (line 115) * Shear: Warping basics. (line 38) * Shell: Command-line interface. (line 6) * Shell auto-complete: Executable names. (line 14) * Shell redirection: Final parameter values. (line 36) * Shell script: GNU Astronomy Utilities 1.0. (line 12) * Shell variables: Installation directory. (line 33) * and : --help. (line 27) * sigma-clipping: Sky value misconceptions. (line 26) * Signal to noise ratio: ImageWarp. (line 21) * Signal to noise ratio <1>: Resampling. (line 21) * Simulating noise: Photon counting noise. (line 66) * Single channel CMYK: Color. (line 40) * size_t: Linked lists. (line 242) * size_t <1>: Linked lists. (line 306) * size_t <2>: Linked lists. (line 344) * Skewed Poisson distribution: Photon counting noise. (line 25) * Sky value: Sky value. (line 6) * Sky value <1>: Sky value. (line 32) * Sky value <2>: Photon counting noise. (line 45) * Software bug: Report a bug. (line 6) * Source code building: Mandatory dependencies. (line 13) * Source code compilation: Mandatory dependencies. (line 13) * Source file navigation: Program source. (line 6) * Source tree: Test scripts. (line 23) * Source, uncompress: Quick start. (line 6) * Spectrum, Fourier: Invoking astconvolve. (line 69) * Spiral galaxies: Hubble visually checks and classifies his catalog. (line 115) * Spline interpolation: Grid interpolation and smoothing. (line 15) * Spread of a point source: PSF. (line 6) * SSD: Configure and build in RAM. (line 12) * SSH: Command-line interface. (line 91) * Standard deviation: Measuring elliptical parameters. (line 38) * Stars, modeling: Stars. (line 6) * Startup scripts: Installation directory. (line 97) * Startup scripts <1>: Generating random numbers. (line 61) * Static document description format: Recognized file types. (line 49) * Static linking: Linking. (line 31) * Statistical analysis: Science and its tools. (line 32) * stdint.h: CFITSIO datatype. (line 42) * Stitch multiple images: ImageCrop. (line 20) * STR: Options. (line 45) * Stray light: SubtractSky. (line 6) * Stream editor, SED: Executable names. (line 60) * Stroustrup, Bjarne: Science and its tools. (line 111) * Stroustrup, Bjarne <1>: Why C. (line 14) * Structure de-reference operator: Mandatory source code files. (line 57) * Structures: Headers. (line 89) * Subaru Telescope: Tiling an image. (line 27) * Submit new tracker item: Report a bug. (line 84) * Suffixes, astronomical data: Arguments. (line 20) * Suffixes, EPS format: Recognized file types. (line 81) * Suffixes, JPEG images: Recognized file types. (line 36) * Suffixes, PDF format: Recognized file types. (line 86) * Suffixes, plain text: Recognized file types. (line 100) * Sum for total flux: Profile magnitude. (line 6) * Superuser, not possible: Installation directory. (line 6) * Support request manager: Report a bug. (line 84) * Symbolic link: Executable names. (line 38) * System Cache: A note on threads. (line 29) * System wide configuration files: System wide. (line 6) * Sérsic index: Galaxies. (line 11) * Sérsic profile: Galaxies. (line 6) * Sérsic, J. L.: Galaxies. (line 11) * Tabs are evil: Coding conventions. (line 156) * Task tracker: Report a bug. (line 97) * Test: Quick start. (line 6) * Test scripts: Test scripts. (line 6) * Tests, only one passes: Known issues. (line 64) * Tests, running: Tests. (line 6) * tests/during-dev.sh: Building and debugging. (line 17) * TeX: Known issues. (line 83) * TeX <1>: Recognized file types. (line 60) * TeX Live: Bootstrapping dependencies. (line 81) * Thread-saftey: FITS functions. (line 209) * Threads, CPU: MakeProfiles options. (line 199) * Tilde expansion as option values: Options. (line 97) * Tile: Tiling an image. (line 6) * tmpfs file system: Configure and build in RAM. (line 23) * tmpfs-config-make: Building and debugging. (line 17) * tmpfs-config-make <1>: Test scripts. (line 23) * Token separation: Command-line. (line 11) * Top processing source file: Mandatory source code files. (line 102) * Top root structure: Mandatory source code files. (line 26) * Tracker: Report a bug. (line 97) * Tracker <1>: Gnuastro project webpage. (line 6) * Trailing space: Coding conventions. (line 151) * Transform image: MakeProfiles. (line 41) * Transformation, affine: Warping basics. (line 85) * Transformation, projective: Warping basics. (line 93) * Truncation radius: Profile magnitude. (line 6) * Tutorial: Tutorials. (line 6) * Type of data: CFITSIO datatype. (line 6) * ui.c, ui.h: Mandatory source code files. (line 78) * Uncompress source: Quick start. (line 6) * Undetected objects: Photon counting noise. (line 45) * Upper limit magnitude: Quantifying data limits. (line 91) * US letter paper size: A4 print book. (line 6) * Usage pattern: --usage. (line 6) * User interface functions: Mandatory source code files. (line 79) * Using CPU threads: Threads in Gnuastro. (line 6) * Using multiple CPU cores: Threads in Gnuastro. (line 6) * Using multiple threads: A note on threads. (line 6) * Values to options: Options. (line 49) * Variance: Measuring elliptical parameters. (line 28) * Variation of background flux: Photon counting noise. (line 60) * Vector graphics: Recognized file types. (line 41) * Version control: Report a bug. (line 27) * Version control <1>: Version controlled source. (line 6) * Version control systems: Optional dependencies. (line 23) * Version number: Version numbering. (line 6) * Versioning: Shared library: Linking. (line 115) * Viewing trackers: Report a bug. (line 97) * Virtual console: Command-line interface. (line 75) * Wall-clock time: A note on threads. (line 19) * WCS: WCSLIB. (line 6) * WCSLIB: WCSLIB. (line 6) * WCSLIB <1>: Invoking astimgwarp. (line 177) * WCSLIB <2>: FITS functions. (line 209) * Weighted average: Convolve. (line 6) * WFC3: ImageWarp. (line 54) * White space character: Configuration file format. (line 11) * Wide Field Camera 3: ImageWarp. (line 54) * Wide Field Camera 3 <1>: Warping basics. (line 51) * William Thomson: Science and its tools. (line 124) * World Coordinate System: WCSLIB. (line 6) * World Coordinate System <1>: Invoking astimgwarp. (line 177) * Writing configuration files: Configuration file format. (line 31) * Wrong output: Report a bug. (line 6) * Wrong results: Report a bug. (line 6) * XDF: Quantifying data limits. (line 56) * Zero-point magnitude: Flux Brightness and magnitude. (line 42) gnuastro-0.2.33-8a3b/doc/gnuastro.info-20000644000175000017500000107210513004464700014544 00000000000000This is gnuastro.info, produced by makeinfo version 6.3 from gnuastro.texi. This book documents version 0.2.33-8a3b of the GNU Astronomy Utilities (Gnuastro). Gnuastro provides various programs and libraries for astronomical data manipulation and analysis. Copyright © 2015-2016 Free Software Foundation, Inc. Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled “GNU Free Documentation Licenseâ€. INFO-DIR-SECTION Astronomy START-INFO-DIR-ENTRY * Gnuastro: (gnuastro). GNU Astronomy Utilities. * help-gnuastro: (gnuastro)help-gnuastro mailing list. Getting help. * bug-gnuastro: (gnuastro)Report a bug. How to report bugs * ConvertType: (gnuastro)ConvertType. Convert different file types. * astconvertt: (gnuastro)Invoking astconvertt. Options to ConvertType. * Convolve: (gnuastro)Convolve. Convolve an input file with kernel. * astconvolve: (gnuastro)Invoking astconvolve. Options to Convolve. * CosmicCalculator: (gnuastro)CosmicCalculator. For cosmological params. * astcosmiccal: (gnuastro)Invoking astcosmiccal. Options to CosmicCalculator. * Header: (gnuastro)Header. Print and manipulate data header info. * astheader: (gnuastro)Invoking astheader. Options to Header. * ImageCrop: (gnuastro)ImageCrop. Crop region(s) from image(s). * astimgcrop: (gnuastro)Invoking astimgcrop. Options to ImageCrop. * Arithmetic: (gnuastro)Arithmetic. Arithmetic operations on pixels. * astarithmetic: (gnuastro)Invoking astarithmetic. Options to Arithmetic. * ImageStatistics: (gnuastro)ImageStatistics. Get image Statistics. * astimgstat: (gnuastro)Invoking astimgstat. Options to ImageStatistics. * ImageWarp: (gnuastro)ImageWarp. Warp an image to a new grid. * astimgwarp: (gnuastro)Invoking astimgwarp. Options to ImageWarp. * MakeCatalog: (gnuastro)MakeCatalog. Make a catalog from labeled image. * astmkcatalog: (gnuastro)Invoking astmkcatalog. Options to MakeCatalog. * MakeNoise: (gnuastro)MakeNoise. Make (add) noise to an image. * astmknoise: (gnuastro)Invoking astmkprof. Options to MakeNoise. * MakeProfiles: (gnuastro)MakeProfiles. Make mock profiles. * astmkprof: (gnuastro)Invoking astmkprof. Options to MakeProfiles. * NoiseChisel: (gnuastro)NoiseChisel. Detect signal in noise. * astnoisechisel: (gnuastro)Invoking astnoisechisel. Options to NoiseChisel. * SubtractSky: (gnuastro)SubtractSky. Find and subtract the sky value. * astsubtractsky: (gnuastro)Invoking astsubtractsky. Options to SubtractSky. * Table: (gnuastro)Table. Read and write FITS binary or ASCII tables. * asttable: (gnuastro)Invoking asttable. Options to Table. END-INFO-DIR-ENTRY  File: gnuastro.info, Node: Invoking astarithmetic, Prev: Arithmetic operators, Up: Arithmetic 6.2.3 Invoking Arithmetic ------------------------- Arithmetic will do pixel to pixel arithmetic operations on the individual pixels of input data and/or numbers. All input data files must have the same dimensions. The general template is: $ astarithmetic [OPTION...] ASTRdata1 [ASTRdata2] OPERATOR ... One line examples: $ astarithmetic 10.32 3.84 - 2.7 pow # will print 155.329 $ astarithmetic 1 image.fits / --out=inverse.fits $ astarithmetic image.fits -1 "*" --out=negative.fits $ astarithmetic image.fits image.fits - --out=skysub.fits \ --hdu=0 --hdu=3 $ astarithmetic image1.fits image2.fits + 2 / --out=average.fits $ astarithmetic image1.fits image2.fits average --out=average.fits $ astarithmetic img1.fits img2.fits img3.fits median \ -h0 -h1 -h2 --out=median.fits If the output is an image, and the ‘--output’ option is not given, automatic output will use the name of the first FITS image encountered to generate an output file name, see *note Automatic output::. Also, output WCS information will be taken from the first input image encountered. If the output is a single number, that number will be printed in the standard output. See *note Reverse polish notation:: for the notation used to mix operands and operators on the command-line. Currently Arithmetic will convert the input image into double precision floating point arrays for the operations. But there are plans to allow it to also operate on integer (labeled or masked) images with bit-wise operators so mask layers can also be manipulated(1). Unless otherwise stated for each operator, blank pixels in the input image will automatically be set as blank in the output. To ignore certain pixels (see *note Blank pixels::), you can specify a mask image, see *note Mask image::. In that case, when reading the first FITS image, all the masked pixels will be changed to a NaN value. Therefore in any further operations with other images, the output for those pixels will always be a NaN (blank pixel value for floating point data type). Currently all the operations in Arithmetic are done in double precision floating point type. However, if none of the input images have this type, the output will be stored as a single precision floating point type. The hyphen (‘-’) can be used both to specify options (see *note Options::) and also to specify a negative number which might be necessary in your arithmetic. In order to enable you to do this, Arithmetic will first parse all the input strings and if the first character after a hyphen is a digit, then that hyphen is temporarily replaced by the vertical tab character which is not commonly used. The arguments are then parsed and these strings will not be specified as an option. Then the given arguments are parsed and any vertical tabs are replaced back with a hyphen so they can be read as negative numbers. So as long as the names of the files you want to work on do not start with a vertical tab followed by a digit, there is no problem. An important consequence of this implementation is that you should not write negative fractions like this: ‘-.3’, instead write them as ‘-0.3’. Without any images, Arithmetic will act like a simple calculator and print the resulting output number on the standard output like the first example above. If you really want such calculator operations on the command-line, AWK (GNU AWK is the most common implementation) is much faster, easier and much more powerful. For example, the numerical one-line example above can be done with the following command. In general AWK is a fantastic tool and GNU AWK has a wonderful manual (). So if you confront situations like this a lot or have to work with large text tables/catalogs, be sure to checkout AWK and simplify your life. $ echo "" | awk '{print (10.32-3.84)^2.7}' 155.329 See *note Common options:: for a review of the options in all Gnuastro programs, the two options related to a mask image are also specified in *note Mask image::. Arithmetic just redefines the ‘--hdu’ option as explained below: ‘-h’ ‘--hdu’ (‘=INT’) Unlike most options in Gnuastro (which will ultimately only have one value for this option), Arithmetic allows ‘--hdu’ to be called multiple times and the value of each invocation will be stored separately (for the unlimited number of input images you would like to use). The order of the values to ‘--hdu’ is very important (if they don’t have the same value!). The order is determined by the order that this option is read: first on the command-line (from left to right), then top-down in each configuration file, see *note Configuration file precedence::. If the number of HDUs is less than the number of input images, Arithmetic will abort and notify you. However, if there are more HDUs than FITS images, there is no problem: they will be used in the given order (every time a FITS image comes up on the stack) and the extra HDUs will be ignored in the end. So there is no problem with having extra HDUs in the configuration files and by default several HDUs with a value of ‘0’ are kept in the system-wide configuration file when you install Gnuastro. ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: Convolve, Next: ImageWarp, Prev: Arithmetic, Up: Image manipulation 6.3 Convolve ============ On an image, convolution can be thought of as a process to blur or remove the contrast in an image. If you are already familiar with the concept and just want to run Convolve, you can jump to *note Convolution kernel:: and *note Invoking astconvolve:: and skip the lengthy introduction on the basic definitions and concepts of convolution. There are generally two methods to convolve an image. The first and more intuitive one is in the “spatial domain†or using the actual image pixel values, see *note Spatial domain convolution::. The second method is when we manipulate the “frequency domainâ€, or work on the magnitudes of the different frequencies that constitute the image, see *note Frequency domain and Fourier operations::. Understanding convolution in the spatial domain is more intuitive and thus recommended if you are just starting to learn about convolution. However, getting a good grasp of the frequency domain is a little more involved and needs some concentration and some mathematical proofs. However, its reward is a faster operation and more importantly a very fundamental understanding of this very important operation. Convolution of an image will generally result in blurring the image because it mixes pixel values. In other words, if the image has sharp differences in neighboring pixel values(1), those sharp differences will become smoother. This has very good consequences in detection of signal in noise for example. In an actual observed image, the variation in neighboring pixel values due to noise can be very high. But after convolution, those variations will decrease and we have a better hope in detecting the possible underlying signal. Another case where convolution is extensively used is in mock images and modeling in general, convolution can be used to simulate the effect of the atmosphere or the optical system on the mock profiles that we create, see *note PSF::. Convolution is a very interesting and important topic in any form of signal analysis (including astronomical observations). So we have thoroughly(2) explained the concepts behind it in the following sub-sections. * Menu: * Spatial domain convolution:: Only using the input image values. * Frequency domain and Fourier operations:: Using frequencies in input. * Spatial vs. Frequency domain:: When to use which? * Convolution kernel:: How to specify the convolution kernel. * Invoking astconvolve:: Options and argument to Convolve. ---------- Footnotes ---------- (1) In astronomy, the only major time we confront such sharp borders in signal are cosmic rays. All other sources of signal in an image are already blurred by the atmosphere or the optics of the instrument. (2) A mathematical will certainly consider this explanation is incomplete and inaccurate. However this text is written for an understanding on the operations that are done on a real (not complex, discrete and noisy) astronomical image, not any general form of abstract function  File: gnuastro.info, Node: Spatial domain convolution, Next: Frequency domain and Fourier operations, Prev: Convolve, Up: Convolve 6.3.1 Spatial domain convolution -------------------------------- The pixels in an input image represent different “spatial†positions, therefore when convolution is done only using the actual input pixel values, we name the process as being done in the “Spatial domainâ€. In particular this is in contrast to the “frequency domain†that we will discuss later in *note Frequency domain and Fourier operations::. In the spatial domain (and in realistic situations where the image and the convolution kernel don’t extend to infinity), convolution is the process of changing the value of one pixel to the _weighted_ average of all the pixels in its _neighborhood_. The ‘neighborhood’ of each pixel (how many pixels in which direction) and the ‘weight’ function (how much each neighboring pixel should contribute depending on its position) are given through a second image which is known as a “kernelâ€(1). * Menu: * Convolution process:: More basic explanations. * Edges in the spatial domain:: Dealing with the edges of an image. ---------- Footnotes ---------- (1) Also known as filter, here we will use ‘kernel’.  File: gnuastro.info, Node: Convolution process, Next: Edges in the spatial domain, Prev: Spatial domain convolution, Up: Spatial domain convolution 6.3.1.1 Convolution process ........................... In convolution, the kernel specifies the weight and positions of the neighbors of each pixel. To find the convolved value of a pixel, the central pixel of the kernel is placed on that pixel. The values of each overlapping pixel in the kernel and image are multiplied by each other and summed for all the kernel pixels. To have one pixel in the center, the sides of the convolution kernel have to be an odd number. This process effectively mixes the pixel values of each pixel with its neighbors, resulting in a blurred image compared to the sharper input image. Formally, convolution is one kind of linear ‘spatial filtering’ in image processing texts. If we assume that the kernel has $2a+1$ and $2b+1$ pixels on each side, the convolved value of a pixel placed at $x$ and $y$ ($C_{x,y}$) can be calculated from the neighboring pixel values in the input image ($I$) and the kernel ($K$) from $$C_{x,y}=\sum_{s=-a}^{a}\sum_{t=-b}^{b}K_{s,t}\times{}I_{x+s,y+t}.$$ Any pixel coordinate that is outside of the image in the equation above will be considered to be zero. When the kernel is symmetric about its center the blurred image has the same orientation as the original image. However, if the kernel is not symmetric, the image will be affected in the opposite manner, this is a natural consequence of the definition of spatial filtering. In order to avoid this we can rotate the kernel about its center by 180 degrees so the convolved output can have the same original orientation. Technically speaking, only if the kernel is flipped the process is known _Convolution_. If it isn’t it is known as _Correlation_. To be a weighted average, the sum of the weights (the pixels in the kernel) have to be unity. This will have the consequence that the convolved image of an object and un-convolved object will have the same brightness (see *note Flux Brightness and magnitude::), which is natural, because convolution should not eat up the object photons, it only disperses them.  File: gnuastro.info, Node: Edges in the spatial domain, Prev: Convolution process, Up: Spatial domain convolution 6.3.1.2 Edges in the spatial domain ................................... In purely ‘linear’ spatial filtering (convolution), there are problems on the edges of the input image. Here we will explain the problem in the spatial domain, see *note Edges in the frequency domain::. The problem originates from the fact that on the edges, in practice(1), the sum of the weights we use on the actual image pixels is not unity. For example, as discussed above, a profile in the center of an image will have the same brightness before and after convolution. However, for a profile on the edge of the image, the brightness (sum of its pixel fluxes within the image, see *note Flux Brightness and magnitude::) will not be equal, some of the flux is going to be ‘eaten’ by the edges. If you ran ‘$ make check’ on the source files of Gnuastro, you can see the this effect by comparing the ‘convolve_frequency.fits’ with ‘convolve_spatial.fits’ in the ‘./tests/’ directory. In the spatial domain, by default, no assumption will be made about pixels outside of the image or any blank pixels in the image, see *note Blank pixels::. The problem explained above will also occur on the sides of blank regions (which might be masked for example). The solution to this edge effect problem is only possible in the spatial domain. We have to discard the assumption that the sum of the kernel pixels is unity during the convolution process(2). So taking $W$ as the sum of the kernel pixels that used non-blank and in-image pixels, the equation in *note Convolution process:: will become: $$C_{x,y}= { \sum_{s=-a}^{a}\sum_{t=-b}^{b}K_{s,t}\times{}I_{x+s,y+t} \over W}.$$ In this manner, objects which are near the sides of the image or blank pixels will also have the same brightness (within the image) before and after convolution. This correction is applied by default in Convolve when convolving in the spatial domain. To disable it, you can use the ‘--noedgecorrection’ option. In the frequency domain, there is no way to avoid this loss of flux near the edges of the image, see *note Edges in the frequency domain::. Note that the edge effect discussed here is different from the one in *note If convolving afterwards::. In making mock images we want to simulate a real observation. In a real observation the images of the galaxies on the sides of the CCD are first blurred by the atmosphere and instrument, then imaged. So light from the parts of a galaxy which are immediately outside the CCD will affect the parts of the galaxy which are covered by the CCD. Therefore in modeling the observation, we have to convolve an image that is larger than the input image by exactly half of the convolution kernel. We can hence conclude that this correction for the edges is only useful when working on actual observed images (where we don’t have any more data on the edges) and not in modeling. ---------- Footnotes ---------- (1) Because we assumed the overlapping pixels outside the input image have a value of zero. (2) ofcourse the sum of the kernel pixels still have to be unity.  File: gnuastro.info, Node: Frequency domain and Fourier operations, Next: Spatial vs. Frequency domain, Prev: Spatial domain convolution, Up: Convolve 6.3.2 Frequency domain and Fourier operations --------------------------------------------- Getting a good grip on the frequency domain is usually not an easy job! So we have decided to give the issue a complete review here. Convolution in the frequency domain (see *note Convolution theorem::) heavily relies on the concepts of Fourier transform (*note Fourier transform::) and Fourier series (*note Fourier series::) so we will be investigating these important operations first. It has become something of a cliché for people to say that the Fourier series “is a way to represent a (wave-like) function as the sum of simple sine waves†(from Wikipedia). However, sines themselves are abstract functions, so this statement really adds no extra layer of physical insight. Before jumping head-first into the equations and proofs, we will begin with a historical background to see how the importance of frequencies actually roots in our ancient desire to see everything in terms of circles. A short review of how the complex plane should be interpreted is then given. Having paved the way with these two basics, we define the Fourier series and subsequently the Fourier transform. The final aim is to explain discrete Fourier transform, however some very important concepts need to be solidified first: The Dirac comb, convolution theorem and sampling theorem. So each of these topics are explained in their own separate sub-sub-section before going on to the discrete Fourier transform. Finally we revisit (after *note Edges in the spatial domain::) the problem of convolution on the edges, but this time in the frequency domain. Understanding the sampling theorem and the discrete Fourier transform is very important in order to be able to pull out valuable science from the discrete image pixels. Therefore we have included the mathematical proofs and figures so you can have a clear understanding of these very important concepts. * Menu: * Fourier series historical background:: Historical background. * Circles and the complex plane:: Interpreting complex numbers. * Fourier series:: Fourier Series definition. * Fourier transform:: Fourier Transform definition. * Dirac delta and comb:: Dirac delta and Dirac comb. * Convolution theorem:: Derivation of Convolution theorem. * Sampling theorem:: Sampling theorem (Nyquist frequency). * Discrete Fourier transform:: Derivation and explanation of DFT. * Fourier operations in two dimensions:: Extend to 2D images. * Edges in the frequency domain:: Interpretation of edge effects.  File: gnuastro.info, Node: Fourier series historical background, Next: Circles and the complex plane, Prev: Frequency domain and Fourier operations, Up: Frequency domain and Fourier operations 6.3.2.1 Fourier series historical background ............................................ Ever since the ancient times, the circle has been (and still is) the simplest shape for abstract comprehension. All you need is a center point and a radius and you are done. All the points on a circle are at a fixed distance from the center. However, the moment you try to connect this elegantly simple and beautiful abstract construct (the circle) with the real world (for example compute its area or its circumference), things become really hard (ideally, impossible) because the irrational number $\pi$ gets involved. The key to understanding the Fourier series (thus the Fourier transform and finally the Discrete Fourier Transform) is our ancient desire to express everything in terms of circles or the most exceptionally simple and elegant abstract human construct. Most people prefer to say the same thing in a more ahistorical manner: to break a function into sines and cosines. As the term “ancient†in the previous sentence implies, Jean-Baptiste Joseph Fourier (1768 – 1830 A.D.) was not the first person to do this. The main reason we know this process by his name today is that he came up with an ingenious method to find the necessary coefficients (radius of) and frequencies (“speed†of rotation on) the circles for any generic (integrable) function. [image src="gnuastro-figures/epicycles.png" alt="Middle ages epicycles along with two demonstrations of breaking a generic function using epicycles." text="../gnuastro-figures//epicycles.png"] Figure 6.1: Epicycles and the Fourier series. Left: A demonstration of Mercury’s epicycles relative to the “center of the world†by Qutb al-Din al-Shirazi (1236 – 1311 A.D.) retrieved from Wikipedia (https://commons.wikimedia.org/wiki/File:Ghotb2.jpg). Middle (https://commons.wikimedia.org/wiki/File:Fourier_series_square_wave_circles_animation.gif) and Right: How adding more epicycles (or terms in the Fourier series) will approximate functions. The right (https://commons.wikimedia.org/wiki/File:Fourier_series_sawtooth_wave_circles_animation.gif) animation is also available. Like most aspects of mathematics, this process of interpreting everything in terms of circles, began for astronomical purposes. When astronomers noticed that the orbit of Mars and other outer planets, did not appear to be a simple circle (as everything should have been in the heavens). At some point during their orbit, the revolution of these planets would become slower, stop, go back a little (in what is known as the retrograde motion) and then continue going forward again. The correction proposed by Ptolemy (90 – 168 A.D.) was the most agreed upon. He put the planets on Epicycles or circles whose center itself rotates on a circle whose center is the earth. Eventually, as observations became more and more precise, it was necessary to add more and more epicycles in order to explain the complex motions of the planets(1). *note Figure 6.1: epicycle.(Left) shows an example depiction of the epicycles of Mercury in the late 13th century. Of course we now know that if they had abdicated the Earth from its throne in the center of the heavens and allowed the Sun to take its place, everything would become much simpler and true. But there wasn’t enough observational evidence for changing the “professional consensus†of the time to this radical view suggested by a small minority(2). So the pre-Galilean astronomers chose to keep Earth in the center and find a correction to the models (while keeping the heavens a purely “circular†order). The main reason we are giving this historical background which might appear off topic is to give historical evidence that while such “approximations†do work and are very useful for pragmatic reasons (like measuring the calendar from the movement of astronomical bodies). They offer no physical insight. The astronomers who were involved with the Ptolemaic world view had to add a huge number of epicycles during the centuries after Ptolemy in order to explain more accurate observations. Finally the death knell of this world-view was Galileo’s observations with his new instrument (the telescope). So the physical insight, which is what Astronomers and Physicists are interested in (as opposed to Mathematicians and Engineers who just like proving and optimizing or calculating!) comes from being creative and not limiting our selves to such approximations. Even when they work. ---------- Footnotes ---------- (1) See the Wikipedia page on “Deferent and epicycle†for a more complete historical review. (2) Aristarchus of Samos (310 – 230 B.C.) appears to be one of the first people to suggest the Sun being in the center of the universe. This approach to science (that the standard model is defined by consensus) and the fact that this consensus might be completely wrong still applies equally well to our models of particle physics and cosmology today.  File: gnuastro.info, Node: Circles and the complex plane, Next: Fourier series, Prev: Fourier series historical background, Up: Frequency domain and Fourier operations 6.3.2.2 Circles and the complex plane ..................................... Before going onto the derivation, it is also useful to review how the complex numbers and their plane relate to the circles we talked about above. The two schematics in the middle and right of *note Figure 6.1: epicycle. show how a 1D function of time can be made using the 2D real and imaginary surface. Seeing the animation in Wikipedia will really help in understanding this important concept. At each point in time, we take the vertical coordinate of the point and use it to find the value of the function at that point in time. *note Figure 6.2: iandtime. shows this relation with the axes marked. Leonhard Euler(1) (1707 – 1783 A.D.) showed that the complex exponential ($e^{iv}$ where $v$ is real) is periodic and can be written as: $e^{iv}=\cos{v}+isin{v}$. Therefore $e^{iv+2\pi}=e^{iv}$. Later, Caspar Wessel (mathematician and cartographer 1745 – 1818 A.D.) showed how complex numbers can be displayed as vectors on a plane. Euler’s identity might seem counter intuitive at first, so we will try to explain it geometrically (for a more physical insight). On the real-imaginary 2D plane (like the left hand plot in each box of *note Figure 6.2: iandtime.), multiplying a number by $i$ can be interpretted as rotating the point by $90$ degrees (for example the value $3$ on the real axis becomes $3i$ on the imaginary axis). On the other hand, $e\equiv\lim_{n\rightarrow\infty}(1+{1\over n})^n$, therefore, defining $m\equiv nu$, we get: $$e^{u}=\lim_{n\rightarrow\infty}\left(1+{1\over n}\right)^{nu} =\lim_{n\rightarrow\infty}\left(1+{u\over nu}\right)^{nu} =\lim_{m\rightarrow\infty}\left(1+{u\over m}\right)^{m}$$ Taking $u\equiv iv$ the result can be written as a generic complex number (a function of $v$): $$e^{iv}=\lim_{m\rightarrow\infty}\left(1+i{v\over m}\right)^{m}=a(v)+ib(v)$$ For $v=\pi$, a nice geometric animation of going to the limit can be seen on Wikipedia (https://commons.wikimedia.org/wiki/File:ExpIPi.gif). We see that $\lim_{m\rightarrow\infty}a(\pi)=-1$, while $\lim_{m\rightarrow\infty}b(\pi)=0$, which gives the famous $e^{i\pi}=-1$ equation. The final value is the real number $-1$, however the distance of the polygon points traversed as $m\rightarrow\infty$ is half the circumference of a circle or $\pi$, showing how $v$ in the equation above can be interpretted as an angle in units of radians and therefore how $a(v)=cos(v)$ and $b(v)=sin(v)$. Since $e^{iv}$ is periodic (let’s assume with a period of $T$), it is more clear to write it as $v\equiv{2{\pi}n\over T}t$ (where $n$ is an integer), so $e^{iv}=e^{i{2{\pi}n\over T}t}$. The advantage of this notation is that the period ($T$) is clearly visible and the frequency ($2{\pi}n \over T$, in units of 1/cycle) is defined through the integer $n$. In this notation, $t$ is in units of “cycleâ€s. As we see from the examples in *note Figure 6.1: epicycle. and *note Figure 6.2: iandtime, for each constituting frequency, we need a respective ‘magnitude’ or the radius of the circle in order to accurately approximate the desired 1D function. The concepts of “period†and “frequency†are relatively easy to grasp when using temporal units like time because this is how we define them in every-day life. However, in an image (astronomical data), we are dealing with spatial units like distance. Therefore, by one “period†we mean the _distance_ at which the signal is identical and frequency is defined as the inverse of that spatial “periodâ€. The complex circle of *note Figure 6.2: iandtime. can be thought of the Moon rotating about Earth which is rotating around the Sun; so the “Real (signal)†axis shows the Moon’s position as seen by a distant observer on the Sun as time goes by. Because of the scalar (not having any direction or vector) nature of time, *note Figure 6.2: iandtime. is easier to understand in units of time. When thinking about spatial units, mentally replace the “Time (sec)†axis with “Distance (meters)â€. Because length has direction and is a vector, visualizing the rotation of the imaginary circle and the advance along the “Distance (meters)†axis is not as simple as temporal units like time. [image src="gnuastro-figures/iandtime.png" text="../gnuastro-figures//iandtime.eps"] Figure 6.2: Relation between the real (signal), imaginary ($i\equiv\sqrt{-1}$) and time axes at two snapshots of time. ---------- Footnotes ---------- (1) Other forms of this equation were known before Euler. For example in 1707 A.D. (the year of Euler’s birth) Abraham de Moivre (1667 – 1754 A.D.) showed that $(\cos{x}+i\sin{x})^n=\cos(nx)+i\sin(nx)$. In 1714 A.D., Roger Cotes (1682 – 1716 A.D. a colleague of Newton who proofread the second edition of Principia) showed that: $ix=\ln(\cos{x}+i\sin{x})$.  File: gnuastro.info, Node: Fourier series, Next: Fourier transform, Prev: Circles and the complex plane, Up: Frequency domain and Fourier operations 6.3.2.3 Fourier series ...................... In astronomical images, our variable (brightness, or number of photo-electrons, or signal to be more generic) is recorded over the 2D spatial surface of a camera pixel. However to make things easier to understand, here we will assume that the signal is recorded in 1D (assume one row of the 2D image pixels). Also for this section and the next (*note Fourier transform::) we will be talking about the signal before it is digitized or pixelated. Let’s assume that we have the continuous function $f(l)$ which is integrable in the interval $[l_0, l_0+L]$ (always true in practical cases like images). Take $l_0$ as the position of the first pixel in the assumed row of the image and $L$ as the width of the image along that row. The units of $l_0$ and $L$ can be in any spatial units (for example meters) or an angular unit (like radians) multiplied by a fixed distance which is more common. To approximate $f(l)$ over this interval, we need to find a set of frequencies and their corresponding ‘magnitude’s (see *note Circles and the complex plane::). Therefore our aim is to show $f(l)$ as the following sum of periodic functions: $$f(l)=\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}n\over L}l} $$ Note that the different frequencies ($2{\pi}n/L$, in units of cycles per meters for example) are not arbitrary. They are all integer multiples of the fundamental frequency of $\omega_0=2\pi/L$. Recall that $L$ was the length of the signal we want to model. Therefore, we see that the smallest possible frequency (or the frequency resolution) in the end, depends on the length we observed the signal or $L$. In the case of each dimension on an image, this is the size of the image in the respective dimension. The frequencies have been defined in this “harmonic†fashion to insure that the final sum is periodic outside of the $[l_0, l_0+L]$ interval too. At this point, you might be thinking that the sky is not periodic with the same period as my camera’s view angle. You are absolutely right! The important thing is that since your camera’s observed region is the only region we are “observing†and will be using, the rest of the sky is irrelevant; so we can safely assume the sky is periodic outside of it. However, this working assumption will haunt us later in *note Edges in the frequency domain::. The frequencies are thus determined by definition. So all we need to do is to find the coefficients ($c_n$), or magnitudes, or radii of the circles for each frequency which is identified with the integer $n$. Fourier’s approach was to multiply both sides with a fixed term: $$f(l)e^{-i{2{\pi}m\over L}l}=\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}(n-m)\over L}l} $$ where $m>0$(1). We can then integrate both sides over the observation period: $$\int_{l_0}^{l_0+L}f(l)e^{-i{2{\pi}m\over L}l}dl =\int_{l_0}^{l_0+L}\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}(n-m)\over L}l}dl=\displaystyle\sum_{n=-\infty}^{\infty}c_n\int_{l_0}^{l_0+L}e^{i{2{\pi}(n-m)\over L}l}dl $$ Both $n$ and $m$ are positive integers. Also, we know that a complex exponential is periodic so after one period ($L$) it comes back to its starting point. Therefore $\int_{l_0}^{l_0+L}e^{2{\pi}k/L}dl=0$ for any $k>0$. However, when $k=0$, this integral becomes: $\int_{l_0}^{l_0+T}e^0dt=\int_{l_0}^{l_0+T}dt=T$. Hence since the integral will be zero for all $n{\neq}m$, we get: $$\displaystyle\sum_{n=-\infty}^{\infty}c_n\int_{l_0}^{l_0+T}e^{i{2{\pi}(n-m)\over L}l}dl=Lc_m $$ The origin of the axis is fundamentally an arbitrary position. So let’s set it to the start of the image such that $l_0=0$. So we can find the “magnitude†of the frequency $2{\pi}m/L$ within $f(l)$ through the relation: $$c_m={1\over L}\int_{0}^{L}f(l)e^{-i{2{\pi}m\over L}l}dl $$ ---------- Footnotes ---------- (1) We could have assumed $m<0$ and set the exponential to positive, but this is more clear.  File: gnuastro.info, Node: Fourier transform, Next: Dirac delta and comb, Prev: Fourier series, Up: Frequency domain and Fourier operations 6.3.2.4 Fourier transform ......................... In *note Fourier series::, we had to assume that the function is periodic outside of the desired interval with a period of $L$. Therefore, assuming that $L\rightarrow\infty$ will allow us to work with any function. However, with this approximation, the fundamental frequency ($\omega_0$) or the frequency resolution that we discussed in *note Fourier series:: will tend to zero: $\omega_0\rightarrow0$. In the equation to find $c_m$, every $m$ represented a frequency (multiple of $\omega_0$) and the integration on $l$ removes the dependence of the right side of the equation on $l$, making it only a function of $m$ or frequency. Let’s define the following two variables: $$\omega{\equiv}m\omega_0={2{\pi}m\over L}$$ $$F(\omega){\equiv}Lc_m$$ The equation to find the coefficients of each frequency in *note Fourier series:: thus becomes: $$F(\omega)=\int_{-\infty}^{\infty}f(l)e^{-i{\omega}l}dl. $$ The function $F(\omega)$ is thus the _Fourier transform_ of $f(l)$ in the frequency domain. So through this transformation, we can find (analyze) the magnitudes of the constituting frequencies or the value in the frequency space(1) of our spatial input function. The great thing is that we can also do the reverse and later synthesize the input function from its Fourier transform. Let’s do it: with the approximations above, multiply the right side of the definition of the Fourier Series (*note Fourier series::) with $1=L/L=({\omega_0}L)/(2\pi)$: $$f(l)={1\over 2\pi}\displaystyle\sum_{n=-\infty}^{\infty}Lc_ne^{{2{\pi}in\over L}l}\omega_0={1\over 2\pi}\displaystyle\sum_{n=-\infty}^{\infty}F(\omega)e^{i{\omega}l}\Delta\omega $$ To find the right most side of this equation, we renamed $\omega_0$ as $\Delta\omega$ because it was our resolution, $2{\pi}n/L$ was written as $\omega$ and finally, $Lc_n$ was written as $F(\omega)$ as we defined above. Now, as $L\rightarrow\infty$, $\Delta\omega\rightarrow0$ so we can write: $$f(l)={1\over 2\pi}\int_{-\infty}^{\infty}F(\omega)e^{i{\omega}l}d\omega $$ Together, these two equations provide us with a very powerful set of tools that we can use to process (analyze) and recreate (synthesize) the input signal. Through the first equation, we can break up our input function into its constituent frequencies and analyze it, hence it is also known as _analysis_. Using the second equation, we can synthesize or make the input function from the known frequencies and their magnitudes. Thus it is known as _synthesis_. Here, we symbolize the Fourier transform (analysis) and its inverse (synthesis) of a function $f(l)$ and its Fourier Transform $F(\omega)$ as ${\cal F}[f]$ and ${\cal F}^{-1}[F]$. ---------- Footnotes ---------- (1) As we discussed before, this ‘magnitude’ can be interpreted as the radius of the circle rotating at this frequency in the epicyclic interpretation of the Fourier series, see *note Figure 6.1: epicycle. and *note Figure 6.2: iandtime.  File: gnuastro.info, Node: Dirac delta and comb, Next: Convolution theorem, Prev: Fourier transform, Up: Frequency domain and Fourier operations 6.3.2.5 Dirac delta and comb ............................ The Dirac $\delta$ (delta) function (also known as an impulse) is the way that we convert a continuous function into a discrete one. It is defined to satisfy the following integral: $$\int_{-\infty}^{\infty}\delta(l)dl=1$$ When integrated with another function, it gives that function’s value at $l=0$: $$\int_{-\infty}^{\infty}f(l)\delta(l)dt=f(0)$$ An impulse positioned at another point (say $l_0$) is written as $\delta(l-l_0)$: $$\int_{-\infty}^{\infty}f(l)\delta(l-l_0)dt=f(l_0)$$ The Dirac $\delta$ function also operates similarly if we use summations instead of integrals. The Fourier transform of the delta function is: $${\cal F}[\delta(l)]=\int_{-\infty}^{\infty}\delta(l)e^{-i{\omega}l}dl=e^{-i{\omega}0}=1$$ $${\cal F}[\delta(l-l_0)]=\int_{-\infty}^{\infty}\delta(l-l_0)e^{-i{\omega}l}dl=e^{-i{\omega}l_0}$$ From the definition of the Dirac $\delta$ we can also define a Dirac comb (${\rm III}_P$) or an impulse train with infinite impulses separated by $P$: $${\rm III}_P(l)\equiv\displaystyle\sum_{k=-\infty}^{\infty}\delta(l-kP) $$ $P$ is chosen to represent “pixel width†later in *note Sampling theorem::. Therefore the Dirac comb is periodic with a period of $P$. We have intentionally used a different name for the period of the Dirac comb compared to the input signal’s length of observation that we showed with $L$ in *note Fourier series::. This difference is highlighted here to avoid confusion later when these two periods are needed together in *note Discrete Fourier transform::. The Fourier transform of the Dirac comb will be necessary in *note Sampling theorem::, so let’s derive it. By its definition, it is periodic, with a period of $P$, so the Fourier coefficients of its Fourier Series (*note Fourier series::) can be calculated within one period: $${\rm III}_P=\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}n\over P}l}$$ We can now find the $c_n$ from *note Fourier series::: $$c_n={1\over P}\int_{-P/2}^{P/2}\delta(l)e^{-i{2{\pi}n\over P}l} ={1\over P}\quad\quad \rightarrow \quad\quad {\rm III}_P={1\over P}\displaystyle\sum_{n=-\infty}^{\infty}e^{i{2{\pi}n\over P}l} $$ So we can write the Fourier transform of the Dirac comb as: $${\cal F}[{\rm III}_P]=\int_{-\infty}^{\infty}{\rm III}_Pe^{-i{\omega}l}dl ={1\over P}\displaystyle\sum_{n=-\infty}^{\infty}\int_{-\infty}^{\infty}e^{-i(\omega-{2{\pi}n\over P})l}dl={1\over P}\displaystyle\sum_{n=-\infty}^{\infty}\delta\left(\omega-{2{\pi}n\over P}\right) $$ In the last step, we used the fact that the complex exponential is a periodic function, that $n$ is an integer and that as we defined in *note Fourier transform::, $\omega{\equiv}m\omega_0$, where $m$ was an integer. The integral will be zero for any $\omega$ that is not equal to $2{\pi}n/P$, a more complete explanation can be seen in *note Fourier series::. Therefore, while in the spatial domain the impulses had spacing of $P$ (meters for example), in the frequency space, the spacing between the different impulses are $2\pi/P$ cycles per meters.  File: gnuastro.info, Node: Convolution theorem, Next: Sampling theorem, Prev: Dirac delta and comb, Up: Frequency domain and Fourier operations 6.3.2.6 Convolution theorem ........................... The convolution (shown with the $\ast$ operator) of the two functions $f(l)$ and $h(l)$ is defined as: $$c(l)\equiv[f{\ast}h](l)=\int_{-\infty}^{\infty}f(\tau)h(l-\tau)d\tau $$ See *note Convolution process:: for a more detailed physical (pixel based) interpretation of this definition. The Fourier transform of convolution ($C(\omega)$) can be written as: $$ C(\omega)=\int_{-\infty}^{\infty}[f{\ast}h](l)e^{-i{\omega}l}dl= \int_{-\infty}^{\infty}f(\tau)\left[\int_{-\infty}^{\infty}h(l-\tau)e^{-i{\omega}l}dl\right]d\tau $$ To solve the inner integral, let’s define $s{\equiv}l-\tau$, so that $ds=dl$ and $l=s+\tau$ then the inner integral becomes: $$\int_{-\infty}^{\infty}h(l-\tau)e^{-i{\omega}l}dl= \int_{-\infty}^{\infty}h(s)e^{-i{\omega}(s+\tau)}ds=e^{-i{\omega}\tau}\int_{-\infty}^{\infty}h(s)e^{-i{\omega}s}ds=H(\omega)e^{-i{\omega}\tau} $$ where $H(\omega)$ is the Fourier transform of $h(l)$. Substituting this result for the inner integral above, we get: $$C(\omega)=H(\omega)\int_{-\infty}^{\infty}f(\tau)e^{-i{\omega}\tau}d\tau=H(\omega)F(\omega)=F(\omega)H(\omega) $$ where $F(\omega)$ is the Fourier transform of $f(l)$. So multiplying the Fourier transform of two functions individually, we get the Fourier transform of their convolution. The convolution theorem also proves a relation between the convolutions in the frequency space. Let’s define: $$D(\omega){\equiv}F(\omega){\ast}H(\omega)$$ Applying the inverse Fourier Transform or synthesis equation (*note Fourier transform::) to both sides and following the same steps above, we get: $$d(l)=f(l)h(l)$$ Where $d(l)$ is the inverse Fourier transform of $D(\omega)$. We can therefore re-write the two equations above formally as the convolution theorem: $$ {\cal F}[f{\ast}h]={\cal F}[f]{\cal F}[h] $$ $$ {\cal F}[fh]={\cal F}[f]\ast{\cal F}[h] $$ Besides its usefulness in blurring an image by convolving it with a given kernel, the convolution theorem also enables us to do another very useful operation in data analysis: to match the blur (or PSF) between two images taken with different telescopes/cameras or under different atmospheric conditions. This process is also known as de-convolution. Let’s take $f(l)$ as the image with a narrower PSF (less blurry) and $c(l)$ as the image with a wider PSF which appears more blurred. Also let’s take $h(l)$ to represent the kernel that should be convolved with the sharper image to create the more blurry image. Above, we proved the relation between these three images through the convolution theorem. But there, we assumed that $f(l)$ and $h(l)$ are known (given) and the convolved image is desired. In de-convolution, we have $f(l)$ –the sharper image– and $f*h(l)$ –the more blurry image– and we want to find the kernel $h(l)$. The solution is a direct result of the convolution theorem: $$ {\cal F}[h]={{\cal F}[f{\ast}h]\over {\cal F}[f]} \quad\quad {\rm or} \quad\quad h(l)={\cal F}^{-1}\left[{{\cal F}[f{\ast}h]\over {\cal F}[f]}\right] $$ While this works really nice, it has two problems: • If ${\cal F}[f]$ has any zero values, then the inverse Fourier transform will not be a number! • If there is significant noise in the image, then the high frequencies of the noise are going to significantly reduce the quality of the final result. A standard solution to both these problems is the Weiner de-convolution algorithm(1). ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: Sampling theorem, Next: Discrete Fourier transform, Prev: Convolution theorem, Up: Frequency domain and Fourier operations 6.3.2.7 Sampling theorem ........................ Our mathematical functions are continuous, however, our data collecting and measuring tools are discrete. Here we want to give a mathematical formulation for digitizing the continuous mathematical functions so that later, we can retrieve the continuous function from the digitized recorded input. Assuming that we have a continuous function $f(l)$, then we can define $f_s(l)$ as the ‘sampled’ $f(l)$ through the Dirac comb (see *note Dirac delta and comb::): $$f_s(l)=f(l){\rm III}_P=\displaystyle\sum_{n=-\infty}^{\infty}f(l)\delta(l-nP) $$ The discrete data-element $f_k$ (for example, a pixel in an image), where $k$ is an integer, can thus be represented as: $$f_k=\int_{-\infty}^{\infty}f_s(l)dl=\int_{-\infty}^{\infty}f(l)\delta(l-kP)dt=f(kP)$$ Note that in practice, our discrete data points are not found in this fashion. Each detector pixel (in an image for example) has an area and averages the signal it receives over that area, not a mathematical point as the Dirac $\delta$ function defines. However, as long as the variation in the signal over one detector pixel is not significant, this can be a good approximation. Having put this issue to the side, we can now try to find the relation between the Fourier transforms of the un-sampled $f(l)$ and the sampled $f_s(l)$. For a more clear notation, let’s define: $$F_s(\omega)\equiv{\cal F}[f_s]$$ $$D(\omega)\equiv{\cal F}[{\rm III}_P]$$ Then using the Convolution theorem (see *note Convolution theorem::), $F_s(\omega)$ can be written as: $$F_s(\omega)={\cal F}[f(l){\rm III}_P]=F(\omega){\ast}D(\omega)$$ Finally, from the definition of convolution and the Fourier transform of the Dirac comb (see *note Dirac delta and comb::), we get: $$\eqalign{ F_s(\omega) &= \int_{-\infty}^{\infty}F(\omega)D(\omega-\mu)d\mu \cr &= {1\over P}\displaystyle\sum_{n=-\infty}^{\infty}\int_{-\infty}^{\infty}F(\omega)\delta\left(\omega-\mu-{2{\pi}n\over P}\right)d\mu \cr &= {1\over P}\displaystyle\sum_{n=-\infty}^{\infty}F\left( \omega-{2{\pi}n\over P}\right).\cr } $$ $F(\omega)$ was only a simple function, see *note Figure 6.3: samplingfreq.(left). However, from the sampled Fourier transform function we see that $F_s(\omega)$ is the superposition of infinite copies of $F(\omega)$ that have been shifted, see *note Figure 6.3: samplingfreq.(right). From the equation, it is clear that the shift in each copy is $2\pi/P$. [image src="gnuastro-figures/samplingfreq.png" text="../gnuastro-figures//samplingfreq.eps"] Figure 6.3: Sampling causes infinite repetition in the frequency domain. FT is an abbreviation for ‘Fourier transform’. $\omega_m$ represents the maximum frequency present in the input. $F(\omega)$ is only symmetric on both sides of 0 when the input is real (not complex). In general $F(\omega)$ is complex and thus cannot be simply plotted like this. Here we have assumed a real Gaussian $f(t)$ which has produced a Gaussian $F(\omega)$. The input $f(l)$ can have any distribution of frequencies in it. In the example of *note Figure 6.3: samplingfreq.(left), the input consisted of a range of frequencies equal to $\Delta\omega=2\omega_m$. Fortunately as *note Figure 6.3: samplingfreq.(right) shows, the assumed pixel size ($P$) we used to sample this hypothetical function was such that $2\pi/P>\Delta\omega$. The consequence is that each copy of $F(\omega)$ has become completely separate from the surrounding copies. Such a digitized (sampled) data set is thus called _over-sampled_. When $2\pi/P=\Delta\omega$, $P$ is just small enough to finely separate even the largest frequencies in the input signal and thus it is known as _critically-sampled_. Finally if $2\pi/P<\Delta\omega$ we are dealing with an _under-sampled_ data set. In an under-sampled data set, the separate copies of $F(\omega)$ are going to overlap and this will deprive us of recovering high constituent frequencies of $f(l)$. The effects of under-sampling in an image with high rates of change (for example a brick wall imaged from a distance) can clearly be visually seen and is known as _aliasing_. When the input $f(l)$ is composed of a finite range of frequencies, $f(l)$ is known as a _band-limited_ function. The example in *note Figure 6.3: samplingfreq.(left) was a nice demonstration of such a case: for all $\omega<-\omega_m$ or $\omega>\omega_m$, we have $F(\omega)=0$. Therefore, when the input function is band-limited and our detector’s pixels are placed such that we have critically (or over-) sampled it, then we can exactly reproduce the continuous $f(l)$ from the discrete or digitized samples. To do that, we just have to isolate one copy of $F(\omega)$ from the infinite copies and take its inverse Fourier transform. This ability to exactly reproduce the continuous input from the sampled or digitized data leads us to the _sampling theorem_ which connects the inherent property of the continuous signal (its maximum frequency) to that of the detector (the spacing between its pixels). The sampling theorem states that the full (continuous) signal can be recovered when the pixel size ($P$) and the maximum constituent frequency in the signal ($\omega_m$) have the following relation(1): $${2\pi\over P}>2\omega_m$$ This relation was first formulated by Harry Nyquist (1889 – 1976 A.D.) in 1928 and formally proved in 1949 by Claude E. Shannon (1916 – 2001 A.D.) in what is now known as the Nyquist-Shannon sampling theorem. In signal processing, the signal is produced (synthesized) by a transmitter and is received and de-coded (analyzed) by a receiver. Therefore producing a band-limited signal is necessary. In astronomy, we do not produce the shapes of our targets, we are only observers. Galaxies can have any shape and size, therefore ideally, our signal is not band-limited. However, since we are always confined to observing through an aperture, the aperture will cause a point source (for which $\omega_m=\infty$) to be spread over several pixels. This spread is quantitatively known as the point spread function or PSF. This spread does blur the image which is undesirable; however, for this analysis it produces the positive outcome that there will be a finite $\omega_m$. Though we should caution that any detector will have noise which will add lots of very high frequency (ideally infinite) changes between the pixels. However, the coefficients of those noise frequencies are usually exceedingly small. ---------- Footnotes ---------- (1) This equation is also shown in some places without the $2\pi$. Whether $2\pi$ is included or not depends on how you define the frequency  File: gnuastro.info, Node: Discrete Fourier transform, Next: Fourier operations in two dimensions, Prev: Sampling theorem, Up: Frequency domain and Fourier operations 6.3.2.8 Discrete Fourier transform .................................. As we have stated several times so far, the input image is a digitized, pixelated or discrete array of values ($f_s(l)$, see *note Sampling theorem::). The input is not a continuous function. Also, all our numerical calculations can only be done on a sampled, or discrete Fourier transform. Note that $F_s(\omega)$ is not discrete, it is continuous. One way would be to find the analytic $F_s(\omega)$, then sample it at any desired “freq-pixelâ€(1) spacing. However, this process would involve two steps of operations and computers in particular are not too good at analytic operations for the first step. So here, we will derive a method to directly find the ‘freq-pixel’ated $F_s(\omega)$ from the pixelated $f_s(l)$. Let’s start with the definition of the Fourier transform (see *note Fourier transform::): $$F_s(\omega)=\int_{-\infty}^{\infty}f_s(l)e^{-i{\omega}l}dl $$ From the definition of $f_s(\omega)$ (using $x$ instead of $n$) we get: $$\eqalign{ F_s(\omega) &= \displaystyle\sum_{x=-\infty}^{\infty} \int_{-\infty}^{\infty}f(l)\delta(l-xP)e^{-i{\omega}l}dl \cr &= \displaystyle\sum_{x=-\infty}^{\infty} f_xe^{-i{\omega}xP} } $$ Where $f_x$ is the value of $f(l)$ on the point $x$ or the value of the $x$th pixel. As shown in *note Sampling theorem:: this function is infinitely periodic with a period of $2\pi/P$. So all we need is the values within one period: $0<\omega<2\pi/P$, see *note Figure 6.3: samplingfreq. We want $X$ samples within this interval, so the frequency difference between each frequency sample or freq-pixel is $1/XP$. Hence we will evaluate the equation above on the points at: $$\omega={u\over XP} \quad\quad u = 0, 1, 2, ..., X-1$$ Therefore the value of the freq-pixel $u$ in the frequency domain is: $$F_u=\displaystyle\sum_{x=0}^{X-1} f_xe^{-i{ux\over X}} $$ Therefore, we see that for each freq-pixel in the frequency domain, we are going to need all the pixels in the spatial domain(2). If the input (spatial) pixel row is also $X$ pixels wide, then we can exactly recover the $x$th pixel with the following summation: $$f_x={1\over X}\displaystyle\sum_{u=0}^{X-1} F_ue^{i{ux\over X}} $$ When the input pixel row (we are still only working on 1D data) has $X$ pixels, then it is $L=XP$ spatial units wide. $L$, or the length of the input data was defined in *note Fourier series:: and $P$ or the space between the pixels in the input was defined in *note Dirac delta and comb::. As we saw in *note Sampling theorem::, the input (spatial) pixel spacing ($P$) specifies the range of frequencies that can be studied and in *note Fourier series:: we saw that the length of the (spatial) input, ($L$) determines the resolution (or size of the freq-pixels) in our discrete Fourier transformed image. Both result from the fact that the frequency domain is the inverse of the spatial domain. ---------- Footnotes ---------- (1) We are using the made-up word “freq-pixel†so they are not confused with spatial domain “pixelsâ€. (2) So even if one pixel is a blank pixel (see *note Blank pixels::), all the pixels in the frequency domain will also be blank.  File: gnuastro.info, Node: Fourier operations in two dimensions, Next: Edges in the frequency domain, Prev: Discrete Fourier transform, Up: Frequency domain and Fourier operations 6.3.2.9 Fourier operations in two dimensions ............................................ Once all the relations in the previous sections have been clearly understood in one dimension, it is very easy to generalize them to two or even more dimensions since each dimension is by definition independent. Previously we defined $l$ as the continuous variable in 1D and the inverse of the period in its direction to be $\omega$. Let’s show the second spatial direction with $m$ the the inverse of the period in the second dimension with $\nu$. The Fourier transform in 2D (see *note Fourier transform::) can be written as: $$F(\omega, \nu)=\int_{-\infty}^{\infty}\int_{-\infty}^{\infty} f(l, m)e^{-i({\omega}l+{\nu}m)}dl$$ $$f(l, m)=\int_{-\infty}^{\infty}\int_{-\infty}^{\infty} F(\omega, \nu)e^{i({\omega}l+{\nu}m)}dl$$ The 2D Dirac $\delta(l,m)$ is non-zero only when $l=m=0$. The 2D Dirac comb (or Dirac brush! See *note Dirac delta and comb::) can be written in units of the 2D Dirac $\delta$. For most image detectors, the sides of a pixel are equal in both dimensions. So $P$ remains unchanged, if a specific device is used which has non-square pixels, then for each dimension a different value should be used. $${\rm III}_P(l, m)\equiv\displaystyle\sum_{j=-\infty}^{\infty} \displaystyle\sum_{k=-\infty}^{\infty} \delta(l-jP, m-kP) $$ The Two dimensional Sampling theorem (see *note Sampling theorem::) is thus very easily derived as before since the frequencies in each dimension are independent. Let’s take $\nu_m$ as the maximum frequency along the second dimension. Therefore the two dimensional sampling theorem says that a 2D band-limited function can be recovered when the following conditions hold(1): $${2\pi\over P} > 2\omega_m \quad\quad\quad {\rm and} \quad\quad\quad {2\pi\over P} > 2\nu_m$$ Finally, let’s represent the pixel counter on the second dimension in the spatial and frequency domains with $y$ and $v$ respectively. Also let’s assume that the input image has $Y$ pixels on the second dimension. Then the two dimensional discrete Fourier transform and its inverse (see *note Discrete Fourier transform::) can be written as: $$F_{u,v}=\displaystyle\sum_{x=0}^{X-1}\displaystyle\sum_{y=0}^{Y-1} f_{x,y}e^{-i({ux\over X}+{vy\over Y})} $$ $$f_{x,y}={1\over XY}\displaystyle\sum_{u=0}^{X-1}\displaystyle\sum_{v=0}^{Y-1} F_{u,v}e^{i({ux\over X}+{vy\over Y})} $$ ---------- Footnotes ---------- (1) If the pixels are not a square, then each dimension has to use the respective pixel size, but since most imagers have square pixels, we assume so here too  File: gnuastro.info, Node: Edges in the frequency domain, Prev: Fourier operations in two dimensions, Up: Frequency domain and Fourier operations 6.3.2.10 Edges in the frequency domain ...................................... With a good grasp of the frequency domain, we can revisit the problem of convolution on the image edges, see *note Edges in the spatial domain::. When we apply the convolution theorem (see *note Convolution theorem::) to convolve an image, we first take the discrete Fourier transforms (DFT, *note Discrete Fourier transform::) of both the input image and the kernel, then we multiply them with each other and then take the inverse DFT to construct the convolved image. Of course, in order to multiply them with each other in the frequency domain, the two images have to be the same size, so let’s assume that we pad the kernel (it is usually smaller than the input image) with zero valued pixels in both dimensions so it becomes the same size as the input image before the DFT. Having multiplied the two DFTs, we now apply the inverse DFT which is where the problem is usually created. If the DFT of the kernel only had values of 1 (unrealistic condition!) then there would be no problem and the inverse DFT of the multiplication would be identical with the input. However in real situations, the kernel’s DFT has a maximum of 1 (because the sum of the kernel has to be one, see *note Convolution process::) and decreases something like the hypothetical profile of *note Figure 6.3: samplingfreq. So when multiplied with the input image’s DFT, the coefficients or magnitudes (see *note Circles and the complex plane::) of the smallest frequency (or the sum of the input image pixels) remains unchanged, while the magnitudes of the higher frequencies are significantly reduced. As we saw in *note Sampling theorem::, the Fourier transform of a discrete input will be infinitely repeated. In the final inverse DFT step, the input is in the frequency domain (the multiplied DFT of the input image and the kernel DFT). So the result (our output convolved image) will be infinitely repeated in the spatial domain. In order to accurately reconstruct the input image, we need all the frequencies with the correct magnitudes. However, when the magnitudes of higher frequencies are decreased, longer periods (shorter frequencies) will dominate in the reconstructed pixel values. Therefore, when constructing a pixel on the edge of the image, the newly empowered longer periods will look beyond the input image edges and will find the repeated input image there. So if you convolve an image in this fashion using the convolution theorem, when a bright object exists on one edge of the image, its blurred wings will be present on the other side of the convolved image. This is often termed as circular convolution or cyclic convolution. So as long as we are dealing with convolution in the frequency domain, there is nothing we can do about the image edges. The least we can do is to eliminate the ghosts of the other side of the image. So, we add zero valued pixels to both the input image and the kernel in both dimensions so the image that will be convolved has the a size equal to the sum of both images in each dimension. Of course, the effect of this zero-padding is that the sides of the output convolved image will become dark. To put it another way, the edges are going to drain the flux from nearby objects. But at least it is consistent across all the edges of the image and is predictable. In Convolve, you can see the padded images when inspecting the frequency domain convolution steps with the ‘--viewfreqsteps’ option.  File: gnuastro.info, Node: Spatial vs. Frequency domain, Next: Convolution kernel, Prev: Frequency domain and Fourier operations, Up: Convolve 6.3.3 Spatial vs. Frequency domain ---------------------------------- With the discussions above it might not be clear when to choose the spatial domain and when to choose the frequency domain. Here we will try to list the benefits of each. The spatial domain, • Can correct for the edge effects of convolution, see *note Edges in the spatial domain::. • Can operate on blank pixels. • Can be faster than frequency domain when the kernel is small (in terms of the number of pixels on the sides). The frequency domain, • Will be much faster when the image and kernel are both large. As a general rule of thumb, when working on an image of modeled profiles use the frequency domain and when working on an image of real (observed) objects use the spatial domain (corrected for the edges). The reason is that if you apply a frequency domain convolution to a real image, you are going to loose information on the edges and generally you don’t want large kernels. But when you have made the profiles in the image yourself, you can just make a larger input image and crop the central parts to completely remove the edge effect, see *note If convolving afterwards::. Also due to oversampling, both the kernels and the images can become very large and the speed boost of frequency domain convolution will significantly improve the processing time, see *note Oversampling::.  File: gnuastro.info, Node: Convolution kernel, Next: Invoking astconvolve, Prev: Spatial vs. Frequency domain, Up: Convolve 6.3.4 Convolution kernel ------------------------ All the programs that need convolution will need to be given a convolution kernel file and extension. In most cases (other than Convolve, see *note Convolve::) the kernel file name is optional. However, the extension is necessary and must be specified either on the command-line or at least one of the configuration files (see *note Configuration files::). Within Gnuastro, there are two ways to create a kernel image: • MakeProfiles: You can use MakeProfiles to create a parametric (based on a radial function) kernel, see *note MakeProfiles::. By default MakeProfiles will make the Gaussian and Moffat profiles in a separate file so you can feed it into any of the programs. • ConvertType: You can write your own desired kernel into a text file table and convert it to a FITS file with ConvertType, see *note ConvertType::. Just be careful that the kernel has to have an odd number of pixels along its two axes, see *note Convolution process::. All the programs that do convolution will normalize the kernel internally, so if you choose this option, you don’t have to worry about normalizing the kernel. Only within Convolve, there is an option to disable normalization, see *note Invoking astconvolve::. The two options to specify a kernel file name and its extension are shown below. These are common between all the programs that will do convolution. ‘-k’ ‘--kernel’ (‘=STR’) The convolution kernel file name. The ‘BITPIX’ (data type) value of this file can be any standard type and it does not necessarily have to be normalized. Several operations will be done on the kernel image prior to the program’s processing: • It will be converted to floating point type. • All blank pixels (see *note Blank pixels::) will be set to zero. • It will be normalized so the sum of its pixels equal unity. • It will be flipped so the convolved image has the same orientation. This is only relevant if the kernel is not circular. See *note Convolution process::. ‘-U’ ‘--khdu’ (‘=STR’) The convolution kernel HDU. Although the kernel file name is optional, before running any of the programs, they need to have a value for ‘--khdu’ even if the default kernel is to be used. So be sure to keep its value in at least one of the configuration files (see *note Configuration files::). By default, the system configuration file has a value. ‘--fullconvolution’ Ignore the (possible) channels in the mesh grid when doing spatial convolution, see *note Tiling an image::. When applied over a mesh grid, spatial convolution will be done independently on each channel. This is necessary when the noise properties of each channel are different and so the pixels should not be mixed. With this option, all channel information is going to be ignored. Currently this option is not deployed for the frequency space convolutions.  File: gnuastro.info, Node: Invoking astconvolve, Prev: Convolution kernel, Up: Convolve 6.3.5 Invoking Convolve ----------------------- Convolve an input image with a known kernel. The general template for Convolve is: $ astconvolve [OPTION...] ASTRdata One line examples: $ astconvolve --kernel=psf.fits mockimg.fits $ astconvolve --kernel=sharperimage.fits --makekernel\ blurryimage.fits The only argument accepted by Convolve is an input image file. Some of the options are the same between Convolve and some other Gnuastro programs. Therefore, to avoid repetition, they will not be repeated here. For the full list of options shared by all Gnuastro programs, please see *note Common options::. *note Mesh grid options:: lists all the options related to specifying a mesh grid which is currently only used in spatial convolution. Note that here, no interpolation or smoothing is defined, only channels and the mesh size are important. *note Convolution kernel:: lists the the convolution kernel options. It is also possible to specify a mask image for the input. In that case, see *note Mask image::. Here we will only explain the options particular to Convolve. Run Convolve with ‘--help’ in order to see the full list of options Convolve accepts, irrespective of where they are explained in this book. ‘--nokernelflip’ Do not flip the kernel after reading it the spatial domain convolution. This can be useful if the flipping has already been applied to the kernel. ‘--nokernelnorm’ Do not normalize the kernel after reading it, such that the sum of its pixels is unity. ‘-f’ ‘--frequency’ Convolve using discrete Fourier transform in the frequency domain: The Fourier transform of both arrays is first calculated and multiplied. Then the inverse Fourier transform is applied to the product to give the final convolved image. For large images, this process will be more efficient than convolving in the spatial domain. However, the edges of the image will loose some flux, see *note Edges in the spatial domain::. ‘-p’ ‘--spatial’ Convolve in the spatial domain, see *note Convolution process::. ‘--viewfreqsteps’ With this option a file with the initial name of the output file will be created that is suffixed with ‘_freqsteps.fits’, all the steps done to arrive at the final convolved image are saved as extensions in this file. The extensions in order are: 1. The padded input image. In frequency domain convolution the two images (input and convolved) have to be the same size and both should be padded by zeros. 2. The padded kernel, similar to the above. 3. The Fourier spectrum of the forward Fourier transform of the input image. Note that the Fourier transform is a complex operation (and not view able in one image!) So we either have to show the ‘Fourier spectrum’ or the ‘Phase angle’. For the complex number $a+ib$, the Fourier spectrum is defined as $\sqrt{a^2+b^2}$ while the phase angle is defined as $\arctan(b/a)$. 4. The Fourier spectrum of the forward Fourier transform of the kernel image. 5. The Fourier spectrum of the multiplied (through complex arithmetic) transformed images. 6. The inverse Fourier transform of the multiplied image. If you open it, you will see that the convolved image is now in the center, not on one side of the image as it started with (in the padded image of the first extension). If you are working on a mock image which originally had pixels of precisely 0.0, you will notice that in those parts that your convolved profile(s) did not convert, the values are now $\sim10^{-18}$, this is due to floating-point round off errors. Therefore in the final step (when cropping the central parts of the image), we also remove any pixel with a value less than $10^{-17}$. ‘-m’ ‘--makekernel’ (‘=INT’) If this option is called, Convolve will do de-convolution (see *note Convolution theorem::). The image specified by the ‘--kernel’ option is assumed to be the sharper (less blurry) image and the input image is assumed to be the more blurry image. The two images have to be the same size. Some notes to take into account for a good result: Noise has large frequencies which can make the result less reliable for the higher frequencies of the kernel. So all the frequencies which have a spectrum smaller than 0.005 in the frequency domain are set to zero and not divided. This will cause the wings of the final kernel to be flatter than they would ideally be which will make the convolved image result unreliable. The value given to this option will be used as the maximum radius of the kernel. Any pixel in the final kernel that is larger than this distance from the center will be set to zero. • Choose a bright (unsaturated) star and use a region box (with ImageCrop for example, see *note ImageCrop::) that is sufficiently above the noise. • Use ImageWarp (see *note ImageWarp::) to warp the pixel grid so the star’s center is exactly on the center of the central pixel in the cropped image. This will certainly slightly degrade the result, however, it is necessary. If there are multiple good stars, you can shift all of them, then normalize them (so the sum of each star’s pixels is one) and then take their average to decrease this effect. • The shifting might move the center of the star by one pixel in any direction, so crop the central pixel of the warped image to have a clean image for the de-convolution.  File: gnuastro.info, Node: ImageWarp, Next: SubtractSky, Prev: Convolve, Up: Image manipulation 6.4 ImageWarp ============= Image warping is the process of mapping the pixels of one image onto a new pixel grid. This process is sometimes known as transformation, however following the discussion of Heckbert 1989(1) we will not be using that term because it can be confused with only pixel value or flux transformations. Here we specifically mean the pixel grid transformation which is better conveyed with ‘warp’. Image wrapping is a very important step in astronomy, both in observational data analysis and in simulating modeled images. In modeling, warping an image is necessary when we want to apply grid transformations to the initial models, for example in simulating gravitational lensing (Radial warpings are not yet included in ImageWarp). Observational reasons for warping an image are listed below: • *Noise:* Most scientifically interesting targets are inherently faint (have a very low Signal to noise ratio). Therefore one short exposure is not enough to detect such objects that are drowned deeply in the noise. We need multiple exposures so we can add them together and increase the objects’ signal to noise ratio. Keeping the telescope fixed on one field of the sky is practically impossible. Therefore very deep observations have to put into the same grid before adding them. • *Resolution:* If we have multiple images of one patch of the sky (hopefully at multiple orientations) we can warp them to the same grid. The multiple orientations will allow us to ‘guess’ the values of pixels on an output pixel grid that has smaller pixel sizes and thus increase the resolution of the output. This process of merging multiple observations is known as Mosaicing. • *Cosmic rays:* Cosmic rays can randomly fall on any part of an image. If they collide vertically with the camera, they are going to create a very sharp and bright spot that in most cases can be separated easily(2). However, depending on the depth of the camera pixels, and the angle that a cosmic rays collides with it, it can cover a line-like larger area on the CCD which makes the detection using their sharp edges very hard and error prone. One of the best methods to remove cosmic rays is to compare multiple images of the same field. To do that, we need all the images to be on the same pixel grid. • *Optical distortion:* (Not yet included in ImageWarp) In wide field images, the optical distortion that occurs on the outer parts of the focal plane will make accurate comparison of the objects at various locations impossible. It is therefore necessary to warp the image and correct for those distortions prior to the analysis. • *Detector not on focal plane:* In some cases (like the Hubble Space Telescope ACS and WFC3 cameras), the CCD might be tilted compared to the focal plane, therefore the recorded CCD pixels have to be projected onto the focal plane before further analysis. * Menu: * Warping basics:: Basics of coordinate transformation. * Merging multiple warpings:: How to merge multiple matrices. * Resampling:: Warping an image is re-sampling it. * Invoking astimgwarp:: Arguments and options for ImageWarp. ---------- Footnotes ---------- (1) Paul S. Heckbert. 1989. _Fundamentals of Texture mapping and Image Warping_, Master’s thesis at University of California, Berkely. (2) All astronomical targets are blurred with the PSF, see *note PSF::, however a cosmic ray is not and so it is very sharp (it suddenly stops at one pixel).  File: gnuastro.info, Node: Warping basics, Next: Merging multiple warpings, Prev: ImageWarp, Up: ImageWarp 6.4.1 Warping basics -------------------- Let’s take $\left[\matrix{u&v}\right]$ as the coordinates of a point in the input image and $\left[\matrix{x&y}\right]$ as the coordinates of that same point in the output image(1). The simplest form of coordinate transformation (or warping) is the scaling of the coordinates, let’s assume we want to scale the first axis by $M$ and the second by $N$, the output coordinates of that point can be calculated by $$\left[\matrix{x\cr y}\right]= \left[\matrix{Mu\cr Nv}\right]= \left[\matrix{M&0\cr0&N}\right]\left[\matrix{u\cr v}\right]$$ Note that these are matrix multiplications. We thus see that we can represent any such grid warping as a matrix. Another thing we can do with this $2\times2$ matrix is to rotate the output coordinate around the common center of both coordinates. If the output is rotated anticlockwise by $\theta$ degrees from the positive (to the right) horizontal axis, then the warping matrix should become: $$\left[\matrix{x\cr y}\right]= \left[\matrix{ucos\theta-vsin\theta\cr usin\theta+vcos\theta}\right]= \left[\matrix{cos\theta&-sin\theta\cr sin\theta&cos\theta}\right] \left[\matrix{u\cr v}\right] $$ We can also flip the coordinates around the first axis, the second axis and the coordinate center with the following three matrices respectively: $$\left[\matrix{1&0\cr0&-1}\right]\quad\quad \left[\matrix{-1&0\cr0&1}\right]\quad\quad \left[\matrix{-1&0\cr0&-1}\right]$$ The final thing we can do with this definition of a $2\times2$ warping matrix is shear. If we want the output to be sheared along the first axis with $A$ and along the second with $B$, then we can use the matrix: $$\left[\matrix{1&A\cr B&1}\right]$$ To have one matrix representing any combination of these steps, you use matrix multiplication, see *note Merging multiple warpings::. So any combinations of these transformations can be displayed with one $2\times2$ matrix: $$\left[\matrix{a&b\cr c&d}\right]$$ The transformations above can cover a lot of the needs of most coordinate transformations. However they are limited to mapping the point $[\matrix{0&0}]$ to $[\matrix{0&0}]$. Therefore they are useless if you want one coordinate to be shifted compared to the other one. They are also space invariant, meaning that all the coordinates in the image will receive the same transformation. In other words, all the pixels in the output image will have the same area if placed over the input image. So transformations which require varying output pixel sizes like projections cannot be applied through this $2\times2$ matrix either (for example for the tilted ACS and WFC3 camera detectors on board the Hubble space telescope). To add these further capabilities, namely translation and projection, we use the homogeneous coordinates. They were defined about 200 years ago by August Ferdinand Möbius (1790 – 1868). For simplicity, we will only discuss points on a 2D plane and avoid the complexities of higher dimensions. We cannot provide a deep mathematical introduction here, interested readers can get a more detailed explanation from Wikipedia(2) and the references therein. By adding an extra coordinate to a point we can add the flexibility we need. The point $[\matrix{x&y}]$ can be represented as $[\matrix{xZ&yZ&Z}]$ in homogeneous coordinates. Therefore multiplying all the coordinates of a point in the homogeneous coordinates with a constant will give the same point. Put another way, the point $[\matrix{x&y&Z}]$ corresponds to the point $[\matrix{x/Z&y/Z}]$ on the constant $Z$ plane. Setting $Z=1$, we get the input image plane, so $[\matrix{u&v&1}]$ corresponds to $[\matrix{u&v}]$. With this definition, the transformations above can be generally written as: $$\left[\matrix{x\cr y\cr 1}\right]= \left[\matrix{a&b&0\cr c&d&0\cr 0&0&1}\right] \left[\matrix{u\cr v\cr 1}\right]$$ We thus acquired 4 extra degrees of freedom. By giving non-zero values to the zero valued elements of the last column we can have translation (try the matrix multiplication!). In general, any coordinate transformation that is represented by the matrix below is known as an affine transformation(3): $$\left[\matrix{a&b&c\cr d&e&f\cr 0&0&1}\right]$$ We can now consider translation, but the affine transform is still spatially invariant. Giving non-zero values to the other two elements in the matrix above gives us the projective transformation or Homography(4) which is the most general type of transformation with the $3\times3$ matrix: $$\left[\matrix{x'\cr y'\cr w}\right]= \left[\matrix{a&b&c\cr d&e&f\cr g&h&1}\right] \left[\matrix{u\cr v\cr 1}\right]$$ So the output coordinates can be calculated from: $$x={x' \over w}={au+bv+c \over gu+hv+1}\quad\quad\quad\quad y={y' \over w}={du+ev+f \over gu+hv+1}$$ Thus with homography we can change the sizes of the output pixels on the input plane, giving a ‘perspective’-like visual impression. This can be quantitatively seen in the two equations above. When $g=h=0$, the denominator is independent of $u$ or $v$ and thus we have spatial invariance. Homography preserves lines at all orientations. A very useful fact about homography is that its inverse is also a homography. These two properties play a very important role in the implementation of this transformation. A short but instructive and illustrated review of affine, projective and also bi-linear mappings is provided in Heckbert 1989(5). ---------- Footnotes ---------- (1) These can be any real number, we are not necessarily talking about integer pixels here. (2) (3) (4) (5) Paul S. Heckbert. 1989. _Fundamentals of Texture mapping and Image Warping_, Master’s thesis at University of California, Berkely. Note that since points are defined as row vectors there, the matrix is the transpose of the one discussed here.  File: gnuastro.info, Node: Merging multiple warpings, Next: Resampling, Prev: Warping basics, Up: ImageWarp 6.4.2 Merging multiple warpings ------------------------------- In *note Warping basics:: we saw how one basic warping/transformation can be represented with a 3 by 3 matrix. To make more complex warpings these matrices have to be multiplied through matrix multiplication. However matrix multiplication is not commutative, so the order of the set of matrices you use for the multiplication is going to be very important. The first warping should be placed as the left-most matrix. The second warping to the right of that and so on. The second transformation is going to occur on the warped coordinates of the first. As an example for merging a few transforms into one matrix, the multiplication below represents the rotation of an image about a point $[\matrix{U&V}]$ anticlockwise from the horizontal axis by an angle of $\theta$. To do this, first we take the origin to $[\matrix{U&V}]$ through translation. Then we rotate the image, then we translate it back to where it was initially. These three operations can be merged in one operation by calculating the matrix multiplication below: $$\left[\matrix{1&0&U\cr0&1&V\cr{}0&0&1}\right] \left[\matrix{cos\theta&-sin\theta&0\cr sin\theta&cos\theta&0\cr 0&0&1}\right] \left[\matrix{1&0&-U\cr0&1&-V\cr{}0&0&1}\right]$$  File: gnuastro.info, Node: Resampling, Next: Invoking astimgwarp, Prev: Merging multiple warpings, Up: ImageWarp 6.4.3 Resampling ---------------- A digital image is composed of discrete ‘picture elements’ or ‘pixels’. When a real image is created from a camera or detector, each pixel’s area is used to store the number of photo-electrons that were created when incident photons collided with that pixel’s surface area. This process is called the ‘sampling’ of a continuous or analog data into digital data. When we change the pixel grid of an image or warp it as we defined in *note Warping basics::, we have to ‘guess’ the flux value of each pixel on the new grid based on the old grid, or re-sample it. Because of the ‘guessing’, any form of warping on the data is going to degrade the image and mix the original pixel values with each other. So if an analysis can be done on an un-warped data image, it is best to leave the image untouched and pursue the analysis. However as discussed in *note ImageWarp:: this is not possible most of the times, so we have to accept the problem and re-sample the image. In most applications of image processing, it is sufficient to consider each pixel to be a point and not an area. This assumption can significantly speed up the processing of an image and also the simplicity of the code. It is a fine assumption when the signal to noise ratio of the objects are very large. The question will then be one of interpolation because you have multiple points distributed over the output image and you want to find the values at the pixel centers. To increase the accuracy, you might also sample more than one point from within a pixel giving you more points for a more accurate interpolation in the output grid. However, interpolation has several problems. The first one is that it will depend on the type of function you want to assume for the interpolation. For example you can choose a bi-linear or bi-cubic (the ‘bi’s are for the 2 dimensional nature of the data) interpolation method. For the latter there are various ways to set the constants(1). Such functional interpolation functions can fail seriously on the edges of an image. They will also need normalization so that the flux of the objects before and after the warpings are comparable. The most basic problem with such techniques is that they are based on a point while a detector pixel is an area. They add a level of subjectivity to the data (make more assumptions through the functions than the data can handle). For most applications this is fine, but in scientific applications where detection of the faintest possible galaxies or fainter parts of bright galaxies is our aim, we cannot afford this loss. Because of these reasons ImageWarp will not use such interpolation techniques. ImageWarp will do interpolation based on “pixel mixingâ€(2) or “area resamplingâ€. This is also what the Hubble Space Telescope pipeline calls “Drizzlingâ€(3). This technique requires no functions, it is thus non-parametric. It is also the closest we can get (make least assumptions) to what actually happens on the detector pixels. The basic idea is that you reverse-transform each output pixel to find which pixels of the input image it covers and what fraction of the area of the input pixels are covered. To find the output pixel value, you simply sum the value of each input pixel weighted by the overlap fraction (between 0 to 1) of the output pixel and that input pixel. Through this process, pixels are treated as an area not as a point (which is how detectors create the image), also the brightness (see *note Flux Brightness and magnitude::) of an object will be left completely unchanged. If there are very high spatial-frequency signals in the image (for example fringes) which vary on a scale smaller than your output image pixel size, pixel mixing can cause ailiasing(4). So if the input image has fringes, they have to be calculated and removed separately (which would naturally be done in any astronomical application). Because of the PSF no astronomical target has a sharp change in the signal so this issue is less important for astronomical applications, see *note PSF::. ---------- Footnotes ---------- (1) see for a nice introduction. (2) For a graphic demonstration see . (3) (4)  File: gnuastro.info, Node: Invoking astimgwarp, Prev: Resampling, Up: ImageWarp 6.4.4 Invoking ImageWarp ------------------------ The general template for invoking ImageWarp is: $ astimgwarp [OPTIONS...] [matrix.txt] InputImage One line examples: $ astimgwarp matrix.txt image.fits $ astimgwarp --align rawimage.fits $ astimgwarp --scale 1.82 --translate 2.1 image.fits $ astimgwarp --rotate=37.92 --scale=0.8 image.fits $ astimgwarp --matrix=0.2,0,0.4,0,0.2,0.4,0,0,1 image.fits $ astimgwarp --matrix="0.7071,-0.7071 0.7071,0.7071" image.fits ImageWarp can accept two arguments, one (an image) is mandatory if any processing is to be done. An optional argument is a plain text file, which must contain the warp/transform matrix, see *note Warping basics::. When this text file is specified, then all options related to the matrix will be ignored (see below for the options). The general options to all Gnuastro programs (including ImageWarp) can be seen in *note Common options::. To be the most accurate the input image will be converted to double precision floating points and all the processing will be done in this format. By default, in the end, the output image will be converted back to the input image data type. Note that if the input type was not a floating point format, then the floating point output pixels are going to be rounded to the nearest integer (using the ‘round’ function in the C programming language) which can lead to a loss of data. This behavior can be disabled with the ‘--doubletype’ option. The input file and input warping matrix elements are stored in the output’s header. When using options, warps can be specified in a modular form, with options to specify each transformation (for example ‘--rotate’, or ‘--scale’), or directly as a matrix (with ‘--matrix’). If specified together, the latter (direct matrix) will take precedence and all the modular warpings will be ignored. Any number of modular warpings can be specified on the command-line and configuration files. If more than one modular warping is given, all will be merged to create one warping matrix. As described in *note Merging multiple warpings::, matrix multiplication is not commutative, so the order of specifying the modular warpings on the command-line, and/or configuration files makes a difference (see *note Configuration file precedence::). Below, the modular warpings are first listed (see *note Warping basics:: for the definition of each type of warping), then the other ImageWarp options. Based on the FITS standard, integer values are assigned to the center of a pixel and the coordinate [1.0, 1.0] is the center of the bottom left (first) image pixel. So the point [0.0, 0.0] is half a pixel away (in each axis) from the bottom left vertice of the first pixel. The resampling that is done in ImageWarp (see *note Resampling::) is dependent on this coordinate. So correction is done internally. With this resampling, the image must be warped relative to the bottom left vertice of the bottom left pixel and that point should lie at [0.0, 0.0]. So for a correct sampling, the warping center must first be translated by [0.5, 0.5], then the warp should be done and finally, a [-0.5, -0.5] translation should be specified. This correction is done internally in the following cases and can be disabled with the ‘--nofitscorrect’ option. • A 2D matrix is given in a file (as an argument). • A 2D matrix is specified with the ‘--matrix’ option. • When modular warpings are used. ‘-a’ ‘--align’ Align the image and celestial (WCS) axes, such that the vertical image direction (when viewed in SAO ds9) corresponds to the declination and the horizontal axis is the inverse of the Right Ascension (RA). The inverse of the RA is chosen so the image can correspond to what you would actually see on the sky and is common in most survey images. Align is internally treated just like a rotation (‘--rotation’), but uses the input image’s WCS to find the rotation angle. ‘-r’ ‘--rotate’ (‘=FLT’) Rotate the input image by the given angle in degrees. Note that commonly, the WCS structure of the image is set such that the RA is the inverse of the image horizontal axis which increases towards the right in the FITS standard and as viewed by SAO ds9. So the default center for rotation is on the right of the image. If you want to rotate about other points, you have to translate the warping center first (with ‘--translate’) then apply your rotation and then return the center back to the original position (with another call to ‘--translate’,z see *note Merging multiple warpings::. ‘-s’ ‘--scale’ (‘=FLT[,FLT]’) Scale the input image by the given factor. If only one value is given, then both image axes will be scaled with the given value. When two values are given, the first will be used to scale the first axis and the second will be used for the second axis. If you only need to scale one axis, use ‘1’ for the axis you don’t need to scale. ‘-f’ ‘--flip’ (‘=FLT[,FLT]’) Flip the image around the first, second or both axes. The first value specifies a flip on the first axis and the second on the second axis. The values of the option only matter if they are non-zero. If any of the values are zero, that axis is not flipped. So if you want to flip by the second axis only, use ‘--flip=0,1’ (which is equivalent to ‘--flip=0,20’ since it only matters if it is non-zero). ‘-e’ ‘--shear’ (‘=FLT[,FLT]’) Apply a shear to the image along the image axes. If only one value is given, then both image axes will be sheared with the given value. When two values are given, the first will be used to shear the first axis and the second will be used for the second axis. If you only need to shear one axis, use ‘0’ for the axis you don’t need. ‘-t’ ‘--translate’ (‘=FLT[,FLT]’) Apply a translation to the image along the image axes. If only one value is given, then both image axes will be translated with the given value. When two values are given, the first will be used to translate along the first axis and the second will be used for the second axis. If you only need to translate one axis, use ‘0’ for the axis you don’t need. ‘-p’ ‘--project’ (‘=FLT[,FLT]’) Apply a projection to the image along the image axes. If only one value is given, then the projection will be applied on both image axes with the given value. When two values are given, the first will be used for the first axis and the second will be used for the second axis. If you only need projection along one axis, use ‘0’ for the axis you don’t need. ‘-m’ ‘--matrix’ (‘=STR’) The warp/transformation matrix. All the elements in this matrix must be separated by any number of space, tab or comma (<,>) characters. If you want to use the first two, then be sure to wrap the matrix within double quotation marks (<">) so they are not confused with other arguments on the command-line, see *note Options::. This also applies to values in the configuration files, see *note Configuration file format::. The transformation matrix can be either 2 by 2 or 3 by 3 array. In the former case (if a 2 by 2 matrix is given), then it is converted to a 3 by 3 matrix with two translation terms added to correct for the FITS definition of position (see *note Warping basics::, *note Merging multiple warpings::, and the explanations above for more). The determinant of the matrix has to be non-zero and it must not contain any non-number values (for example infinities or NaNs). The elements of the matrix have to be written row by row. So for the general homography matrix of *note Warping basics::, it should be called with ‘--matrix=a,b,c,d,e,f,g,h,1’. ‘--nofitscorrect’ Do not correct for the FITS definition of the pixel center as described in the descriptions above. ‘--hstartwcs’ (‘=INT’) Specify the first header keyword number (line) that should be used to read the WCS information, see the full explanation in *note Invoking astimgcrop::. ‘--hendwcs’ (‘=INT’) Specify the last header keyword number (line) that should be used to read the WCS information, see the full explanation in *note Invoking astimgcrop::. ‘-n’ ‘--nowcscorrection’ Do not correct the WCS information of the input image and save it untouched to the output image. By default the WCS (World Coordinate System) information of the input image is going to be corrected in the output image. WCSLIB will save the input WCS information in the ‘PC’ matrix(1). To correct the WCS, ImageWarp multiplies the ‘PC’ matrix with the inverse of the specified transformation matrix. Also the ‘CRPIX’ point is going to be changed to its correct place in the output image coordinates. This behavior can be disabled with the ‘--nowcscorrection’ option. ‘-z’ ‘--zerofornoinput’ Set output pixels which do not correspond to any input to zero. By default they are set to blank pixel values, see *note Blank pixels::. ‘-b’ ‘--maxblankfrac’ (‘=FLT’) The maximum fractional area of blank pixels over the output pixel. If an output pixel is covered by blank pixels (see *note Blank pixels::) for a larger fraction than the value to this option, the output pixel will be set to a blank pixel its self. When the fraction is lower, the sum of non-blank pixel values over that pixel will be multiplied by the inverse of this fraction to correct for its flux and not cause discontinuities on the edges of blank regions. Note that even with this correction, discontinuities (very low non-blank values touching blank regions in the output image) might arise depending on the transformation and the blank pixels. So if there are blank pixels in the image, a good value to this option has to be found for that particular image and warp. ‘-d’ ‘--doubletype’ By default the output image is going to have the same type as the input image. If this option is called, the output will be in double precision floating point format irrespective of the input data type. When dealing with integer input formats, this option can be useful in checking the results. ---------- Footnotes ---------- (1) Greisen E.W., Calabretta M.R. (2002) Representation of world coordinates in FITS. Astronomy and Astrophysics, 395, 1061-1075.  File: gnuastro.info, Node: SubtractSky, Prev: ImageWarp, Up: Image manipulation 6.5 SubtractSky =============== Raw astronomical images (and even poorly processed images) don’t usually have a uniform ‘sky’ value over their surface prior to processing, see *note Sky value:: for a complete definition of the sky value. However, a uniform sky value over the image is vital for further processing. For ground based images (particularly at longer wavelengths) this can be due to actual variations in the atmosphere. Another cause might be systematic biases in the instrument or prior processing. For example stray light in the telescope/camera or bad flat-fielding or bias subtraction. The latter is a major issue in space based images where the atmosphere is no longer a problem. SubtractSky is a tool to find the sky value and its standard deviation on a grid over the image. The size of the grid will determine how accurately it can account for gradients in the sky value. Such that if the gradient (change of sky value) is too sharp, a smaller grid size has to be chosen. However the results will be most accurate with a larger grid size. * Menu: * Sky value:: Definition of the sky value. * Tiling an image:: Defining a mesh grid on the image. * Mask image:: How to mask pixels for no analysis. * Invoking astsubtractsky:: Options and arguments to SubtractSky.  File: gnuastro.info, Node: Sky value, Next: Tiling an image, Prev: SubtractSky, Up: SubtractSky 6.5.1 Sky value --------------- The discussion here is taken from Akhlaghi and Ichikawa (2015)(1). Let’s assume that all instrument defects – bias, dark and flat – have been corrected and the brightness (see *note Flux Brightness and magnitude::) of a detected object, $O$, is desired. The sources of flux on pixel $i$(2) of the image can be written as follows: • Contribution from the target object, ($O_i$). • Contribution from other detected objects, ($D_i$). • Undetected objects or the fainter undetected regions of bright objects, ($U_i$). • A cosmic ray, ($C_i$). • The background flux, which is defined to be the count if none of the others exists on that pixel, ($B_i$). The total flux in this pixel, $T_i$, can thus be written as: $$T_i=B_i+D_i+U_i+C_i+O_i.$$ By definition, $D_i$ is detected and it can be assumed that it is correctly subtracted, so that $D_i$ can be set to zero. There are also methods to detect and remove cosmic rays (for example, van Dokkum (2001)(3)) enabling us to set $C_i=0$. Note that in practice, $D_i$ and $U_i$ are correlated, because they both directly depend on the detection algorithm and its input parameters. Also note that no detection or cosmic ray removal algorithm is perfect. With these limitations in mind, the observed sky value for this pixel ($S_i$) can be defined as $$S_i=B_i+U_i.$$ Therefore, as the detection process (algorithm and input parameters) becomes more accurate, or $U_i\to0$, the sky value will tend to the background value or $S_i\to B_i$. Therefore, while $B_i$ is an inherent property of the data (pixel in an image), $S_i$ depends on the detection process. Over a group of pixels, for example in an image or part of an image, this equation translates to the average of undetected pixels. With this definition of sky, the object flux in the data can be calculated with $$T_{i}=S_{i}+O_{i} \quad\rightarrow\quad O_{i}=T_{i}-S_{i}.$$ Hence, the more accurately $S_i$ is measured, the more accurately the brightness (sum of pixel values) of the target object can be measured (photometry). Similarly, any under-(over-)estimation in the sky will directly translate to an over(under) estimation of the measured object’s brightness. In the fainter outskirts of an object a very small fraction of the photo-electrons in the pixels actually belong to objects. Therefore even a small over estimation of the sky value will result in the loss of a very large portion of most galaxies. Based on the definition above, the sky value is only correctly found when all the detected objects ($D_i$ and $C_i$) have been removed from the data. * Menu: * Finding the sky value:: How SubtractSky finds the sky value. * Sky value misconceptions:: Sky value misconceptions and wrong approaches. ---------- Footnotes ---------- (1) See the section on sky in Akhlaghi M., Ichikawa. T. (2015). Astrophysical Journal Supplement Series. (2) For this analysis the dimension of the data (image) is irrelevant. So if the data is an image (2D) with width of $w$ pixels, then a pixel located on column $x$ and row $y$ (where all counting starts from zero and (0, 0) is located on the bottom left corner of the image), would have an index: $i=x+y\times{}w$. (3) van Dokkum, P. G. (2001). Publications of the Astronomical Society of the Pacific. 113, 1420.  File: gnuastro.info, Node: Finding the sky value, Next: Sky value misconceptions, Prev: Sky value, Up: Sky value 6.5.1.1 Finding the sky value ............................. This technique to find the sky value in a distribution was initially proposed in Akhlaghi and Ichikawa 2015(1). Note that through the difference of the mode and median we have actually ‘detected’ data in the distribution. However this detection was only based on the total distribution of the data, not its spatial position in each mesh. So we adhere to the definition of Sky value in *note Sky value::. Finding the median is very easy, the main problem is in finding the mode through a robust method. In Appendix C of Akhlaghi and Ichikawa (2015) a new approach to finding the mode in any astronomically relevant distribution is introduced. Even when the mode and median are approximately equal, Cosmic rays can significantly bias the calculation of the average. Even if they are very few. However, usually, Cosmic rays have very sharp boundaries and do not fade away into the noise. Therefore, when the histogram of the distribution is plotted, they are clearly separate from the rest of the data. For example see Figure 15 in Akhlaghi and Ichikawa (2015). In such cases, $\sigma$-clipping is a perfect tool to remove the effect of such objects in the average and standard deviation. See *note Sigma clipping:: for a complete explanation. So after asserting that the mode and median are approximately equal in a mesh (see *note Tiling an image::), convergence-based $\sigma$-clipping is also applied before getting the final sky value and its standard deviation for a mesh. ---------- Footnotes ---------- (1) Akhlaghi M., Ichikawa. T. (2015). Astrophysical Journal Supplement Series.  File: gnuastro.info, Node: Sky value misconceptions, Prev: Finding the sky value, Up: Sky value 6.5.1.2 Sky value misconceptions ................................ As defined in *note Sky value::, the sky value is only accurately defined when the detection algorithm is not significantly reliant on the sky value. In particular its detection threshold. However, most signal-based detection tools (1) used the sky value as a reference to define the detection threshold. So these old techniques had to rely on approximations based on other assumptions about the data. A review of those other techniques can be seen in Appendix A of Akhlaghi and Ichikawa (2015)(2). Since they were extensively used in astronomical data analysis for several decades, such approximations have given rise to a lot of misconceptions, ambiguities and disagreements about the sky value and how to measure it. As a summary, the major methods used until now were an approximation of the mode of the image pixel distribution and $\sigma$-clipping. • To find the mode of a distribution those methods would either have to assume (or find) a certain probability density function (PDF) or use the histogram. But the image pixels can have any distribution, and the histogram results are very inaccurate (there is a large dispersion) and depend on bin-widths. • Another approach was to iteratively clip the brightest pixels in the image (which is known as $\sigma$-clipping, since the reference was found from the image mean and its standard deviation or $\sigma$). See *note Sigma clipping:: for a complete explanation. The problem with $\sigma$-clipping was that real astronomical objects have diffuse and faint wings that penetrate deeply into the noise. So only removing their brightest parts is completely useless in removing the systematic bias an object’s fainter parts cause in the sky value. As discussed in *note Sky value::, the sky value can only be correctly defined as the average of undetected pixels. Therefore all such approaches that try to approximate the sky value prior to detection are ultimately poor approximations. ---------- Footnotes ---------- (1) According to Akhlaghi and Ichikawa (2015), signal-based detection is a detection process that relies heavily on assumptions about the to-be-detected objects. This method was the most heavily used technique prior to the introduction of NoiseChisel in that paper. (2) Akhlaghi M., Ichikawa. T. (2015). Astrophysical Journal Supplement Series.  File: gnuastro.info, Node: Tiling an image, Next: Mask image, Prev: Sky value, Up: SubtractSky 6.5.2 Tiling an image --------------------- Some of the programs in Gnuastro will need to divide the pixels in an image into individual tiles or a mesh grid to be able to deal with gradients. In this section we will explain the concept in detail and how the user can check the grid. In the case of SubtractSky, if the image is completely uniform then one sky value will suffice for the whole image. See *note Sky value:: for the definition of the sky value. Unfortunately though, as discussed in *note SubtractSky::, in most images taken with ground or space-based telescopes the sky value is not uniform. So we have to break the image up into small tiles on a mesh grid, assume the sky value is constant over them and find the sky value on those tiles. Meshes are considered to be a square with a side of ‘--meshsize’ pixels. The best mesh size is directly related to the gradient on the image. In practice we assume that the gradient is not significant over each mesh. So if there is a strong gradient (for example in long wavelength ground based images) or the image is of a crowded area where there isn’t too much blank area, you have to choose a smaller mesh size. A larger mesh will give more pixels and so the scatter in the results will be less. For raw image processing, a simple mesh grid is not sufficient. Raw images are the unprocessed outputs of the camera detectors. Large detectors usually have multiple readout channels each with its own amplifier. For example the Hubble Space Telescope Advanced Camera for Surveys (ACS) has four amplifiers over its full detector area dividing the square field of view to four smaller squares. Ground based image detectors are not exempt, for example each CCD of Subaru Telescope’s Hyper Suprime-Cam camera (which has 104 CCDs) has four amplifiers, but they have the same height of the CCD and divide the width by four parts. The bias current on each amplifier is different, and normally bias subtraction is not accurately done. So even after subtracting the measured bias current, you can usually still identify the boundaries of different amplifiers by eye. See Figure 11(a) in Akhlaghi and Ichikawa (2015) for an example. This results in the final reduced data to have non-uniform amplifier-shaped regions with higher or lower background flux values. Such systematic biases will then propagate to all subsequent measurements we do on the data (for example photometry and subsequent stellar mass and star formation rate measurements in the case of galaxies). Therefore an accurate sky subtraction routine should also be able to account for such biases. To get an accurate result, the mesh boundaries should be located exactly on the amplifier boundaries. Otherwise, some meshes will contain pixels that have been read from two or four different amplifiers. These meshes are going to give very biased results and the amplifier boundary will still be present after sky subtraction. So we define ‘channel’s. A channel is an independent mesh grid that covers one amplifier to ensure that the meshes do not pass the amplifier boundary. They can also be used in subsequent steps as the area used to identify nearby neighbors to interpolate and smooth the final grid, see *note Grid interpolation and smoothing::. The number of channels along each axis can be specified by the user at run time through the command-line ‘--nch1’ and ‘--nch2’ options or in the configuration files, see *note Configuration files::. The area of each channel will then be tiled by meshes of the given size and subsequent processing will be done on those meshes. If the image is processed or the detector only has one amplifier, you can set the number of channels in both axes to 1. Unlike the channel size, that has to be an exact multiple of the image size, the mesh size can be any number. If it is not an exact multiple of the image side, the last mesh (rightest, for the first FITS dimension, and highest for the second when viewed in SAO ds9) will have a different size than the rest. If the remainder of the image size divided by mesh size is larger than a certain fraction (value to ‘--lastmeshfrac’) of the mesh size along each axis, a new (smaller) mesh will be put there instead of a larger mesh. This is done to avoid the last mesh becoming too large compared to the other meshes in the grid. Generally, it is best practice to choose the mesh size such that the last mesh is only a few (negligible) pixels wider or thinner than the rest. The final mesh grid can be seen on the image with the ‘--checkmesh’ option that is available to all programs which use the mesh grid for localized operations. When this option is called, a multi-extension FITS file with a ‘_mesh.fits’ suffix will be created along with the outputs, see *note Automatic output::. The first extension will be the input image. For each mesh grid the image produces, there will be a subsequent extension. Each pixel in the grid extensions is labeled to the mesh that it is part of. You can flip through the extensions to check the mesh sizes and locations compared to the input image. * Menu: * Quantifying signal in a mesh:: Good meshs for gradients. * Grid interpolation and smoothing:: Filling the blank grid elements. * Checking grid values:: Check the values on the grid. * Mesh grid options:: Common options related to the mesh grid.  File: gnuastro.info, Node: Quantifying signal in a mesh, Next: Grid interpolation and smoothing, Prev: Tiling an image, Up: Tiling an image 6.5.2.1 Quantifying signal in a mesh .................................... Noise is characterized with a fixed background value and a certain distribution. For example, for the Gaussian distribution these two are the mean and standard deviation. When we have absolutely no signal and only noise in a data set, the mean, median and mode of the distribution are equal within statistical errors and approximately equal to the background value. For the next paragraph, let’s assume that the background is subtracted and is zero. Data always has a positive value and will never become negative, see Figure 1 in Akhlaghi and Ichikawa (2015). Therefore, as data is buried into the noise, the mean, median and mode shift to the positive. The mean is the fastest in this shift. The median is slower since it is defined based on an ordered distribution and so is not affected by a small (less than half) number of outliers. Finally, the mode is the slowest to shift to the positive. Inverting the argument above provides us with the basis of Gnuastro’s algorithm to quantify the presence of signal in a mesh. Namely, when the mode and median of a distribution are approximately equal, we can argue that there is no significant signal in that mesh. So we can consider the image to be made of a grid and use this argument to ‘detect’ signal in each grid element. The median is defined to be the value of the 0.5 quantile in the image. So the only necessary parameter is the minimum acceptable quantile (smaller than 0.5) for the mode in a mesh that we deem accurate. See *note Mesh grid options:: for an explanation of the options used to customize this behavior. Since there is sufficient signal in the mesh to bias the analysis on that mesh, any grid element whose mode quantile is smaller than the minimum acceptable quantile is usually kept with a blank value and no value is given to it. Finally, when all the grid elements have been checked, we can interpolate over all the empty elements and smooth the final result to find the sky value over the full image. See *note Grid interpolation and smoothing::. Convolving a data set (that contains signal and noise), creates a positive skewness in it depending on the fraction of data present in the distribution and also the convolution kernel. See Section 3.1.1 in Akhlaghi and Ichikawa (2015) and *note Convolution process::. This skewness can be interpreted as an increase in the Signal to noise ratio of the objects buried in the noise. Therefore, to obtain an even better measure of the presence of signal in a mesh, the image can be convolved with a given PSF first. This positive skew will result in more distance between the mode an median thereby enabling a more accurate detection of fainter signal, for example the faint wings of bright stars and galaxies. When convolving over a mesh grid, the pixels in each channel will be treated independently. This can be disabled with the ‘--fullconvolution’ option. See *note Convolution kernel:: for the respective options.  File: gnuastro.info, Node: Grid interpolation and smoothing, Next: Checking grid values, Prev: Quantifying signal in a mesh, Up: Tiling an image 6.5.2.2 Grid interpolation and smoothing ........................................ On some of the grid elements, the desired value will not be found, for example the Sky value in *note Finding the sky value::. This can happen for lots of reasons depending on the job that was to be done on a mesh, for example when a large galaxy is present in the image, no Sky value will be found for the grid elements that lie over it. However, the Sky value should be ‘guessed’ over that part of the image. We cannot just ignore those regions! To fill in such blank grid elements, we use interpolation. Parametric interpolations like bi-linear, bicubic or spline interpolations are not used because they fail terribly on the edges of the image. For example see Figure 16 in Akhlaghi and Ichikawa (2015). They are also prone to cause significant gradients in the image. So to find the interpolated value for each grid element, Gnuastro will look at a certain number of the nearest neighbors. The exact number can be specified through ‘--numnearest’. The median value of those grid elements will be taken as the final value for each mesh. The median is chosen because on the fainter wings of bright objects, the mean can easily become biased. If the number of meshes with a good value is less than the value given to ‘--numnearest’, then the program will abort and notify you. In such cases you can either decrease the value to this option or set less restrictive requirements (for example a smaller ‘--minmodeq’, or larger/smaller meshs) at the expense of less accurate results. By default the process above will occur on all the grid elements, not just the ones that are blank. This is done to avoid biased results on the faint wings of bright galaxies and stars (the PSF). Because their flux penetrates into the noise very slowly, it might not be possible to completely identify that flux and ignore that mesh. Therefore, if interpolation is only done on blank pixels, such false positives can cause a bias in the vicinity of bright objects, particularly after smoothing in the next step. In order to only interpolate over blank meshs and leave the values of the successful meshs untouched, the ‘--interponlyblank’ option can be used. Once all the grid elements are filled, the values given to all the meshs should be smoothed. This is because the median was used in the interpolation. The median is robust in the face of outliers, but there might be strong differences from one grid element to the next. By smoothing the grid, the variation between grid element to grid element will be far less. To smooth the mesh values, Gnuastro uses an average filter. An average filter is just a convolution of the mesh grid (spatial convolution with edge correction) by a kernel with all elements having an equal weight, see *note Convolution process::. The kernel is a square. The length of the kernel edge can be set in units of meshs through the ‘--smoothwidth’ option (which has to be an odd number as with any kernel). If a width of 1 is given for the kernel width, then no smoothing will take place. By default the interpolation and smoothing explained above are done independently on each channel. In some circumstances, it might be preferable to do either one of these two steps on the whole image, independent of the channels. For example when there are gradients over the image and their variation over the image is stronger than the variation caused by the channels. Through the two options ‘--fullinterpolation’ and ‘--fullsmooth’ you can ask for interpolation or smoothing to use all the meshs in the image, not just those in the same channel of a mesh. Note that it is still very important that no mesh contain pixels from two channels. Since the pixels have been assigned to a mesh prior to these steps (see *note Tiling an image::), there is no problem in this regard. Even after smoothing, a simple visual examination of the values given to the pixels in each mesh over the image will give a very ‘boxy’ or pixelated impression. To our eyes it feels that it would be much better if the values could be smoothed in sub-mesh (pixel) scales to obtain a smooth variation. An example is the results of bi-linear and bi-cubic interpolations, see Figure 16 in Akhlaghi and Ichikawa (2015) for several examples. The reasons we are not doing that level of smoothing are two fold: • The difference in value between neighboring meshs is not statistically significant. After smoothing, the variation between the neighboring mesh values will be very small. It does visually appear to be a lot when viewing in image viewers like SAO ds9. This is because such viewers use the minimum and maximum range of all the pixel values as a reference to choose the color given to each pixel. However compared to the standard deviation of the noise in the image, the different values of each mesh are completely negligible. Please confirm this for your self on your own datasets to clearly understand. • Such pixel-based (not mesh-based) interpolation will be very time consuming. Since the difference between the neighboring meshs is statistically negligible, it is simply not worth the time investment.  File: gnuastro.info, Node: Checking grid values, Next: Mesh grid options, Prev: Grid interpolation and smoothing, Up: Tiling an image 6.5.2.3 Checking grid values ............................ Programs that use the mesh grid to calculate some value, also have checking options (that start with ‘--check’). When such options are called, the program will create a specific output file depending on what you want to check. When the operation is done on the meshes, this file shows the values assigned to each mesh grid element. It has three extensions: 1. The value that was initially calculated for each grid element. If a mesh was not successful in providing a value, a NaN value is stored for that mesh. 2. The interpolated values, see *note Grid interpolation and smoothing::. 3. The smoothed values, see *note Grid interpolation and smoothing::. If more than one value is calculated for each mesh (for example the mean and its standard deviation), then each step has that many extensions. By default, these check image outputs have the same size (pixels) as the input image. So all the pixels within a mesh are given the same value. This is useful if you want to later apply these values to the image through another program for example. There is a one to one correspondence between the input image pixels and the grid showing you the mesh values for that pixel. In other situations, the input pixel resolution might not be important for you and you just want to see the relative mesh values over the image. In such cases, you can call the ‘--meshbasedcheck’ option so the check image only has one pixel for each mesh. This image will only be as big as the full mesh grid and there will be no world coordinate system. When the input images are really large, this can make a difference in both the processing of the programs and in viewing the images. Another case when only one pixel for each mesh will be useful is when you might want to display the mesh values in a document and you don’t want the volume of the document (in bytes) to get too high. For example if the mesh sizes are 30 pixels by 30 pixels, then the mesh grid created through this option will take $30\times30=900$ times less space! You can resize the standard output, but the borders between the meshs will be blurred. The best case is to call that program with this option.  File: gnuastro.info, Node: Mesh grid options, Prev: Checking grid values, Up: Tiling an image 6.5.2.4 Mesh grid options ......................... The mesh grid structure defined here (see *note Tiling an image::) is used by more than one program. Therefore in order to avoid repetition, all the options to do with the mesh grid (and are shared by all the programs using it) are listed here. Some programs might define multiple meshs over the image (for example in NoiseChisel, there is a large and a small mesh for different operations, see *note NoiseChisel::), in such cases, the options for each mesh are designated by an appropriate prefix. For example in NoiseChisel the small and large mesh sizes are specified through the ‘--smeshsize’ and ‘--lmeshsize’ respectively. Both these options are similar to the ‘--meshsize’ option explained below, but for their respective grid. Note that the short option name might also differ. If such options exist in a program, they are listed in the ‘Invoking ProgramName’ section within the list of options. ‘-s’ ‘--meshsize’ (‘=INT’) The size of each mesh, see *note Tiling an image::. If the width of all channels are not an exact multiple of the specified size, then the last mesh on each axis will have a different size to cover the full channel. ‘-a’ ‘--nch1’ (‘=INT’) The number of channels along the first FITS axis (horizontal when viewed in SAO ds9). If the length of the image is not an exact multiple of this number, then the program will stop. You can use ImageCrop (*note ImageCrop::) to trim off or add some pixels (blank pixels if added, see *note Blank pixels::) to the image if it is not an exact multiple. ‘-b’ ‘--nch2’ (‘=INT’) The number of channels along the second FITS axis, (vertical when viewed in SAO ds9). Similar to ‘--nch1’. ‘-L’ ‘--lastmeshfrac’ (‘=FLT’) Fraction of extra area on the last (rightest on the first FITS axis and highest/top on the second) mesh, to define a new (smaller) one. See *note Tiling an image::. ‘--checkmesh’ An image with suffix ‘_mesh.fits’ will be created for you to check the mesh grid, see *note Tiling an image::. The input image will be the first extension, followed by an extension, where each pixel is labeled (number starting from zero) by the ID of the mesh it belongs to. If the program uses multiple mesh grids, the output will have more than two extensions. By flipping through the extensions, you can check the positioning and size of the meshs. ‘-d’ ‘--mirrordist’ (‘=FLT’) The distance beyond the mirror point (in units of the error in the mirror point) to check for finding the mode in each mesh. This is part of the process to quantify the presence of signal in a mesh, see *note Quantifying signal in a mesh::. See appendix C in Akhlaghi and Ichikawa (2015) for a complete explanation of the mode-finding algorithm. The value to this option is shown as $\alpha$ in that appendix. ‘-Q’ ‘--minmodeq’ (‘=FLT’) The minimum acceptable quantile for the mode of each mesh. The median is on the 0.5 quantile of the image and as long as we have positive signal (all astronomically relevant observations), the mode will be less than the median. The sky value is only found on meshes where the median and mode are approximately the same, see *note Sky value::. ‘--interponlyblank’ Only interpolate the blank pixels. By default, interpolation will happen on all the mesh grids, not just the blank ones. See *note Grid interpolation and smoothing::. ‘-n’ ‘--numnearest’ (‘=INT’) The number of nearest grid elements with a successful sky value to use for interpolating over blank mesh elements (those that had a significant contribution of signal), see *note Grid interpolation and smoothing::. ‘--fullinterpolation’ Do interpolation irrespective of the channels in the image, see *note Grid interpolation and smoothing::. ‘-T’ ‘--smoothwidth’ (‘=INT’) The width of the average filter kernel used to smooth the interpolated image in units of pixels. See *note Grid interpolation and smoothing::. If this option is given a value of 1 (one), then no smoothing will be done. ‘--fullsmoothing’ Do smoothing irrespective of the channels in the image, see *note Grid interpolation and smoothing::. ‘--meshbasedcheck’ Store the fixed value in each mesh in one check image pixel, see *note Checking grid values::. Note that this image has no world coordinate system.  File: gnuastro.info, Node: Mask image, Next: Invoking astsubtractsky, Prev: Tiling an image, Up: SubtractSky 6.5.3 Mask image ---------------- All of the programs in Gnuastro that do processing on the input data can also account for masked pixels. Particularly in raw data processing, there are usually a set of pixels in the image that should not be included in any analysis. For example saturated pixels on the centers of bright objects, or the edges of the image which received no data and were only used for bias calculation. The detectors or the very early processing that is done on raw images clearly identifies such cases and usually assigns an integer (or flag or mask value) to those pixels. Pixels that are good for processing usually have a zero value in the mask image. It goes without saying that the two images have to have the same size. Note that if the mask image has blank pixels, then they act like pixels with non-zero values and will be masked (see *note Blank pixels::). The integer values in the mask images are usually sums of powers of two. Each power of two has a specific meaning and since the sum of two different sets of powers of two are never equal, each mask value identifies a set of different properties for each masked pixels. For some analysis, some masked properties might not be a problem. Therefore a pixel that only has that property should be included. In such cases, you can use bit flags to keep some of the powers of two and remove the rest. The individual Gnuastro programs do not consider these issues. Therefore, if some masked pixels should be included in the analysis, it is best to use another tool to set the appropriate mask pixel values to zero prior to running the analysis program. We are working on such a program as part of Gnuastro. If the data type (‘BITPIX’) of the input mask image is not an integer type, the programs will print a warning, but continue on with the analysis. This usually happens because of a mistake in specifying the file or the HDU. The programs that accept a mask image, all share the options below. Any masked pixels will receive a NaN value (or a blank pixel, see *note Blank pixels::) in the final output of those programs. In fact, another way to notify any of the Gnuastro programs to not use a certain set of pixels in a data set is to set those pixels equal to appropriate blank pixel value for the type of the image, *note Blank pixels::. ‘-M’ ‘--mask’ (‘=STR’) Mask image file name. If this option is not given and the ‘--mhdu’ option has a different value from ‘--hdu’, then the input image name will be used. If a name is specified on the command-line or in any of the configuration files, it will be used. If the program doesn’t get any mask file name, it will use all the non-blank (see *note Blank pixels::) pixels in the image. Therefore, specifying a mask file name in any of the configuration files is not mandatory. ‘-H’ ‘--mhdu’ (‘=STR’) The mask image header name or number. Similar to the ‘--hdu’ option, see *note Common options::. Like ‘--mask’, this option does not have to be included in the configuration file or the command-line. However, if it is present on either of them, it will be used.  File: gnuastro.info, Node: Invoking astsubtractsky, Prev: Mask image, Up: SubtractSky 6.5.4 Invoking SubtractSky -------------------------- SubtractSky will find the sky value on a grid in an image and subtract it. The executable name is ‘astsubtractsky’ with the following general template: $ astsubtractsky [OPTION ...] Image One line examples: $ astsubtractsky image.fits $ astsubtractsky --hdu=0 --mhdu=1 image.fits $ astsubtractsky --nch1=2 --nch2=2 image.fits $ astsubtractsky --mask=maskforimage.fits image.fits The only required input to SubtractSky is the input data file that currently has to be only a 2D image. But in the future it might be useful to use it for 1D or 3D data too. Any pixels in the image with a blank value will be ignored in the analysis, see *note Blank pixels::. Alternatively a mask can be specified which indicates pixels to not be used (see ‘--mask’ and ‘--mhdu’). The common options to all Gnuastro programs can be seen in *note Common options:: and input data formats are explained in *note Arguments::. SubtractSky uses a mesh grid to tile the image. This enables it to deal with possible gradients, see *note Tiling an image::. The mesh grid options are common to all the programs using it, and are listed in *note Mesh grid options::. In order to ignore some pixels during the analysis, you can specify a mask image, see *note Mask image:: for an explanation and the relevant options. For a more accurate result, a kernel file name can be specified so the image is first convolved, see *note Quantifying signal in a mesh::, see *note Convolution kernel:: for the kernel related options. The ‘--kernel’ option is not mandatory and if not specified anywhere prior to running, the original image will be used. Please run SubtractSky with the ‘--help’ option to list all the recognized options, irrespective of which part of the book they are fully explained in. ‘-u’ ‘--sigclipmultip’ (‘=FLT’) The multiple of the standard deviation to clip from the distribution in $\sigma$-clipping. This is necessary to remove the effect of cosmic rays, see *note Sky value:: and *note Sigma clipping::. ‘-t’ ‘--sigcliptolerance’ (‘=FLT’) The tolerance of sigma clipping. If the fractional change in the standard deviation before and after $\sigma$-clipping is less than the value given to this option, $\sigma$-clipping will stop, see *note Sigma clipping::. ‘--checksky’ A two extension FITS image ending with ‘_smooth.fits’ will be created showing how the interpolated sky value is smoothed. ‘--checkskystd’ In the interpolation and sky checks above, include the sky standard deviation too. By default, only the sky value is shown in all the checks. However with this option, an extension will be added showing how the standard deviation on each mesh is finally found too.  File: gnuastro.info, Node: Image analysis, Next: Modeling and fittings, Prev: Image manipulation, Up: Top 7 Image analysis **************** Astronomical images contain very valuable information, the tools in this section can help in extracting and quantifying that information. For example calculating image statistics, or finding the sky value or detecting objects within an image. * Menu: * ImageStatistics:: Calculate main image statistics. * NoiseChisel:: Detect objects in an image. * MakeCatalog:: Catalog from input and labeled images.  File: gnuastro.info, Node: ImageStatistics, Next: NoiseChisel, Prev: Image analysis, Up: Image analysis 7.1 ImageStatistics =================== The distribution of pixel values in an image can give us valuable information about the image, for example if it is a positively skewed distribution, we can see that there is significant data in the image. If the distribution is roughly symmetric, we can tell that there is no significant data in the image. On the other hand, in some measurements that we do on the image, we might need to know the certain statistical parameters of the image. For example, if we have run a detection algorithm on an image, and we want to see how accurate it was, one method is to calculate the average of the undetected pixels and see how reasonable it is (if detection is done correctly, the average of undetected pixels should be approximately equal to the background value, see *note Sky value::). ImageStatistics is built for precisely such situations. * Menu: * Histogram and Cumulative Frequency Plot:: Basic definitions. * Sigma clipping:: Definition of $\sigma$-clipping * Mirror distribution:: Used for finding the mode. * Invoking astimgstat:: Arguments and options to ImageStatistics.  File: gnuastro.info, Node: Histogram and Cumulative Frequency Plot, Next: Sigma clipping, Prev: ImageStatistics, Up: ImageStatistics 7.1.1 Histogram and Cumulative Frequency Plot --------------------------------------------- Histograms and the cumulative frequency plots are both used to study the distribution of data. The histogram is mainly easier to understand for the untrained eye, while the cumulative frequency plot is more accurate, but needs a good level of experience for interpretation. A histogram shows the number of data points which lie within pre-defined intervals (bins). It is used to get a general view of the distribution and its shape. The width of the bins is one of the most important parameters for a histogram. In the limiting case that the bin-widths tend to zero (and assuming there is data for each bin), then the normalized histogram would show the probability distribution function of the distribution. Normalizing a histogram means to divide the number of data points in each bin by the total number of data. In the cumulative frequency plot of a distribution, the x axis is the sorted data values and the y axis is the index of each data in the sorted distribution. Unlike a histogram, a cumulative frequency plot does not involve intervals or bins. This makes it less prone to any sort of bias or error that a given bin-width would have on the analysis. When a larger number of the data points have roughly the same value, then the cumulative frequency plot will become steep in that vicinity. This occurs because on the x axis (data values), there is little change while on the y axis the indexes constantly increase. Normalizing a cumulative frequency plot means to divide each index (y axis) by the total number of data points. Unlike the histogram which has a limited number of bins, ideally the cumulative frequency plot should have one point for every data point. Even in small images (for example a $200\times200$) this will result in an unreasonably larger number of points to plot (40000)! So when the cumulative frequency plot of an image is stored in a text file, it is best to only store its value on a certain number of points (intervals) rather than the whole data. The number of points to use for the final plot can be specified with the ‘--cfpnum’ option. Note that the interval’s lower value is considered to be part of each interval, but its larger value is not. Formally, an interval between a and b is represented by [a, b). This is true for all the intervals except the last one. The last interval is closed or [a, b].  File: gnuastro.info, Node: Sigma clipping, Next: Mirror distribution, Prev: Histogram and Cumulative Frequency Plot, Up: ImageStatistics 7.1.2 Sigma clipping -------------------- Let’s assume that you have pure noise (centered on zero) with a clear Gaussian distribution, see *note Photon counting noise::. Now let’s assume you add very bright objects (signal) on the image which have a very sharp boundary. By a sharp boundary, we mean that there is a clear cutoff at the place the objects finish. In other words, at their boundaries, the objects do not fade away into the noise. In such a case, when you plot the histogram (see *note Histogram and Cumulative Frequency Plot::) of the distribution, the pixels relating to those objects will be clearly separate from pixels that belong to parts of the image that did not have data. In the cumulative frequency plot, you would observe a long flat region were for a certain range of data (x axis), there is no increase in the index (y axis). In cases like the above, $\sigma$-clipping is a very useful tool to remove the effect (bias) of such forms of signal from the distribution. In astronomical applications, cosmic rays (when they collide at a near normal incidence angle) are a very good example of such signals. The tracks they leave behind in the image are perfectly immune to the blurring caused by the atmosphere and the aperture. They are also very energetic and so their borders are usually clearly separated from the surrounding noise. So $\sigma$-clipping is very useful in removing their effect on the data. See Figure 15 in Akhlaghi and Ichikawa (2015). $\sigma$-clipping is the very simple iteration below. In each iteration, the range of input data might decrease and so when the data in the image have the conditions above, they will be removed. The criteria to stop the iteration will be discussed below. 1. Calculate the mean, standard deviation ($\sigma$) and median ($m$) of a distribution. 2. Remove all points that are smaller or larger than $m\pm\alpha\sigma$. The reason the median is used as a reference and not the mean is that the mean is too significantly affected by the presence of signal, while the median is less affected, see *note Finding the sky value::. As you can tell from this algorithm, besides the condition above (that the signal have clear high signal to noise boundaries) $\sigma$-clipping is only useful when the signal does not cover more than half of the full data set. If they do, then the median will lie over the signal and sigma clipping might remove the pixels with no signal. In the literature researchers use either one of two criteria to stop this iteration above: • When a certain number of iterations has taken place. • When the new measured standard deviation is within a certain tolerance level of the old one. The tolerance level is defined by: $$\sigma_{old}-\sigma_{new} \over \sigma_{new}$$ The standard deviation is heavily influenced by the presence of outliers. Therefore the fact that it stops changing between two iterations is a sign that we have successfully removed outliers. Note that in each clipping, the dispersion in the distribution is either less or equal. So $\sigma_{old}\geq\sigma_{new}$. Other objects in astronomical data analysis like galaxies and stars are blurred by the atmosphere and the telescope aperture. Galaxies in particular do not appear to have a clear high signal to noise cutoff at all. Therefore $\sigma$-clipping will not be useful in removing their effect on the data. In astronomy, it is only useful for removing the effect of Cosmic rays.  File: gnuastro.info, Node: Mirror distribution, Next: Invoking astimgstat, Prev: Sigma clipping, Up: ImageStatistics 7.1.3 Mirror distribution ------------------------- The mirror distribution of a data set was defined in Appendix C of Akhlaghi and Ichikawa (2015). It is best visualized by mentally placing a mirror on the histogram of a distribution at any point within the distribution (which we call the mirror point). Through the ‘--mirrorquant’ in ImageStatistics, you can check the mirror of a distribution when the mirror is placed on any given quantile. The mirror distribution is plotted along with the input distribution both as histograms and cumulative frequency plots, see *note Histogram and Cumulative Frequency Plot::. Unlike the rest of the histograms and cumulative frequency plots in ImageStatistics, the text files created with the ‘--mirrorquant’ and ‘--checkmode’ will contain 3 columns. The first is the horizontal axis similar to all other histograms and cumulative frequency plots. The second column shows the respective value for the actual data distribution and the third shows the value for the mirror distribution. The value for each bin of both histogram is divided by the maximum of both. For the cumulative frequency plot, the value in each bin is divided by the maximum number of elements. So one of the cumulative frequency plots reaches the maximum vertical axis of 1. The outputs will have the ‘_mirrorhist.txt’ and ‘_mirrorcfp.txt’ suffixes respectively. You can use a simple Python script like the one below to display the histograms and cumulative frequency plots in one plot: #! /usr/bin/env python3 # Import the necessary modules: import sys import numpy as np import matplotlib.pyplot as plt # Load the two files: a=np.loadtxt(sys.argv[1]+"_mirrorhist.txt") b=np.loadtxt(sys.argv[1]+"_mirrorcfp.txt") # Calculate the bin width: w=a[1,0]-a[0,0] # Plot the two histograms and cumulative frequency plots: plt.bar(a[:,0], a[:,1], width=w, color="blue", linewidth=0, alpha=0.6) plt.bar(a[:,0], a[:,2], width=w, color="green", linewidth=0, alpha=0.4) plt.plot(b[:,0], b[:,1], linewidth=2, color="blue") plt.plot(b[:,0], b[:,2], linewidth=2, color="green") # Write the axis labels: plt.ylim([0,np.amax(a[:,1])]) plt.xlim([np.amin(a[:,0]),np.amax(a[:,0])]) # Save the output to any name from the command-line: plt.savefig(sys.argv[1]+"_plot.pdf") The output format can be anything that Python’s Matplotlib recognizes (for example png or jpg are also acceptable). So, if your input data file name was ‘input.fits’, and you want to see how its mirror distribution would look like if the mirror was placed at the 0.8 quantile (or the value which is above 80 percent of your data) you can run the following sequence of commands to see the combined cumulative frequency plot and histogram together in one PDF file. Let’s assume you have put the Python script above into the file ‘mirrorplot.py’. The second command makes the Python script an executable file. $ ls input.fits mirrorplot.py $ chmod +x mirrorplot.py $ astimgstat input.fits --nohist --nocfp --mirrorquant=0.8 $ ls input.fits input_mirrorcfp.txt input_mirrorhist.txt mirrorplot.py $ ./mirrorplot.py input By default, the range of the mirror distribution is set to the 0.01 quantile of the image to 2 times the distance of the mode to that point. This is done so that the mode (which will have a value of zero in this plot) is positioned exactly on 1/3rd point of the x axis plot. The number of bins is the same value as the ‘--histnumbins’ option. Alternatively, through the option ‘--histrangeformirror’, the histogram properties set with the ‘--histmin’ and ‘--histmax’ can be used. In these mirror plots, the mirror value is going to have the value of zero and one of the bins is going to start at zero (if ‘--histrangeformirror’ is called, the given ranges will also shift accordingly).  File: gnuastro.info, Node: Invoking astimgstat, Prev: Mirror distribution, Up: ImageStatistics 7.1.4 Invoking ImageStatistics ------------------------------ ImageStatistics will print the major statistical measures of an image’s pixel value distribution. The executable name is ‘astimgstat’ with the following general template $ astimgstat [OPTION ...] InputImage.fits One line examples: $ astimgstat input.fits $ astimgstat animage.fits --ignoremin --nohist $ astimgstat anotherimage.fits --mask=detectionlabels.fits --mhdu=1 If ImageStatistics is to do any data processing, an input image should be provided with the recognized extensions as input data, see *note Arguments::. See *note Common options:: for the list of options that are shared by all programs. All the main statistical operations have their specific set of options. If a string is given to the ‘--output’ option, it is used as the base name for the generated files. Without this option, the input image name is used as the name-base. Some of the options are necessary and if they are not included in the configuration file, ImageStatistics will not run, see *note Configuration files::. However, for some others this is not so: ‘--histmin’, ‘--histmax’, ‘--histquant’, ‘--cfpmin’, ‘--cfpmax’, ‘--cfpquant’. These are options to do with the range of values in the histogram and cumulative frequency plots. If no value is given for these options when ImageStatistics is about to start processing the data, then the full data range will be used. Such that the minimum image value will be set for the minimums and the maximum image value will be used for the maximum. The Mask name and HDU are also not mandatory in the configuration file. By default, in verbose mode (1), along with a short summary of the basic data statistics, a simple ASCII histogram will also be printed. This can be useful for a very quick and general view of the distribution. An example verbose output of ImageStatistics on one of the ‘$ make check’ outputs can be seen below: $ astimgstat ./tests/convolve_spatial_warped_noised.fits \ --histquant=0.05 ImageStatistics started on AAA BBB CC DD:EE:FF GGGG - Input read: ./tests/convolve_spatial_warped_noised.fits (hdu: 0) -- Number of points 10000 -- Minimum -38.2066 -- Maximum 1268.72 -- Sum 154927 -- Mean 15.4927 -- Standard deviation 60.5407 -- Median 4.82691 -- Mode (quantile, value) 0.4335, 2.90301 -- Mode symmetricity and its cutoff value 0.5909, 17.2507 -- ASCII histogram in the range: -13.912957 -- 65.058487: | * * | ******** | ********* ** | ************** | ****************** | ******************** | *********************** |*************************** |****************************** |***************************************** |************************************************************ |------------------------------------------------------------ - Sigma clipping results (Median, Mean, STD, Number): - 4.00 times sigma by convergence (tolerance: 0.2000): 1: 4.826907, 15.492665, 60.540707, 10000 2: 4.665353, 10.117773, 27.793823, 9881 3: 4.433090, 7.458610, 18.510950, 9715 4: 4.216213, 6.176818, 15.231371, 9575 5: 4.088199, 5.679162, 14.183748, 9502 - 4.00 sigma-clipping 5 times: 1: 4.826907, 15.492665, 60.540707, 10000 2: 4.665353, 10.117773, 27.793823, 9881 3: 4.433090, 7.458610, 18.510950, 9715 4: 4.216213, 6.176818, 15.231371, 9575 5: 4.088199, 5.679162, 14.183748, 9502 ImageStatistics finished in: 0.006964 (seconds) ‘-M’ ‘--mask’ (‘=STR’) The file name of a mask image. If this option is not given on the command-line or in the configuration files and ‘--mhdu’ is not given or is identical to ‘--hdu’, then no mask image will be used. ‘-H’ ‘--mhdu’ (‘=STR’) The header name of the mask extension. ‘-r’ ‘--ignoremin’ Ignore all data elements that have a value equal to the minimum value in the image. In practice this is like masking those pixels, their values will not be used. ‘-l’ ‘--lowerbin’ Set the first column of the histogram and cumulative frequency plots to the lower interval boundary. By default (without calling this option), the central interval value is used. ‘--onebinvalue’ (‘=FLT’) Make sure that one bin starts with the value to this option. In practice, this will shift the bins used to find the histogram and cumulative frequency plot such that one bin’s lower interval becomes this value. For example when the histogram range includes negative values, but the data doesn’t. If zero is somewhere between one bin, then the viewers of the plot(s) will think negative data is also present. By setting ‘--onebinvalue=0’, you can make sure that the viewers of the histogram will not be confused. Note that by default, the first row of the histogram and cumulative frequency plot show the central values of each bin. So in the example above you will not see the 0.000. To see it, add the ‘--lowerbin’ option to show the lower value of each bin. If you don’t care about the bin positions within the specified range you can set the value to this option to a Not-a-Number (NaN) value on the command-line (‘--onebinvalue=nan’) or in the configuration files with a ‘nan’ following the option name. If the value is not within the specified bin range, it will be ignored. ‘--noasciihist’ Do not show an ASCII plot on the command-line. ‘--mirrorquant’ (‘=FLT’) quantile to put the mirror. A value between 0 and 1. See *note Mirror distribution:: for a complete explanation. Outputs two files with suffixes ‘_mirrorhist.txt’ and ‘_mirrorcfp.txt’. ‘--checkmode’ The mode of the data is found by comparing the input data distribution with its mirror distribution. If this option is called, the mirror distribution’s histogram and cumulative frequency plots will be saved in to plain text files ending with ‘_modehist.txt’ and ‘_modecfp.txt’. See the explanation for *note Mirror distribution:: for more details about these two files and how you can easily plot the outputs. This option only works when when ImageStatistics is in verbose mode. Since otherwise the mode is not calculated. To draw the plots you can use the script in *note Mirror distribution::. Just change the appended suffixes in the two calls to ‘np.loadtxt’ in the Python script. ‘--histrangeformirror’ Use ‘--histmin’ and ‘--histmax’ for the range of the mirror distributions (which are produced with the ‘--mirrorquant’ and ‘--checkmode’ options). *Histogram:* The stored histogram is stored in a text file ending with ‘_hist.txt’. ‘--nohist’ Do not calculate or save the histogram. ‘--normhist’ Make a normalized histogram, see *note Histogram and Cumulative Frequency Plot::. ‘--maxhistone’ Divide all histogram bins by the number in the bin with the most data points. This is very useful if you want to plot the histogram along with a normalized cumulative frequency plot in one plot. Note that if the histogram numbers are important in showing along with the cumulative frequency plot, you can use ‘--maxcfpeqmaxhist’, see below. ‘-n’ ‘--histnumbins’ (‘=INT’) The number of bins in the histogram. Note that in practice, this is also equivalent to the number of rows in the output text file. ‘-i’ ‘--histmin’ (‘=FLT’) The minimum value to use in the histogram. If ‘--histquant’ is given, then any value given ‘--histmin’ or ‘--histmax’ is ignored. ‘-x’ ‘--histmax’ (‘=FLT’) The maximum value to use in the histogram. Similar to ‘--histmin’. ‘-Q’ ‘--histquant’ (‘=FLT’) Set the range of the histogram based on the image quantile. So ‘--histquant=0.05’ is given, all the data from the 0.05 quantile to 0.95 quantile will be used in the histogram. This is useful when there is a small number of outliers in the image. Note that if this option is given, any (possible) value given to ‘--histmin’ or ‘--histmax’ are ignored. *Cumulative Frequency Plot:* The cumulative frequency plot will be stored in a text file ending with ‘_cfp.txt’. To be more realistic, the average of the indexs in each interval is used as the second column, see *note Histogram and Cumulative Frequency Plot::. ‘--nocfp’ Do not calculate or store the cumulative frequency plot. ‘--normcfp’ Normalize the cumulative frequency plot, see *note Histogram and Cumulative Frequency Plot::. ‘--maxcfpeqmaxhist’ Set the maximum cumulative frequency plot value to the maximum value in the histogram (if it is to be created). This is a useful in plotting the histogram and cumulative frequency plots together when the histogram numbers are important. ‘--cfpsimhist’ Set the range of the cumulative frequency plot and the number of points to store to the same range as the histogram. If the two are to be plotted together, this is very useful, since the first axis (column) of the two will become identical. ‘-p’ ‘--cfpnum’ (‘=INT’) The number of points to store the cumulative frequency plot. They will be evenly distributed between the range of pixel values. ‘-a’ ‘--cfpmin’ (‘=FLT’) The minimum value to use for the cumulative pixel value range. If ‘--cfpquant’ is given, then any value given ‘--cfpmin’ or ‘--cfpmax’ is ignored. ‘-n’ ‘--cfpmax’ (‘=FLT’) The maximum value to use for the cumulative pixel value range. Similar to ‘--cfpmin’. ‘-U’ ‘--cfpquant’ (‘=FLT’) Similar to ‘--histquant’ but for the cumulative frequency plot. *$\sigma$-clipping:* The result of each iteration of $\sigma$-clipping will be printed in the terminal for both types of sigma clipping: A certain number of times and convergence of the standard deviation. ‘--nosigclip’ If this option is called, no $\sigma$-clipping will take place. ‘-u’ ‘--sigclipmultip’ (‘=FLT’) The multiple of the standard deviation above which to clip. This value is demonstrated by $\alpha$ in *note Sigma clipping::. ‘-t’ ‘--sigcliptolerance’ (‘=FLT’) If the fractional difference of the standard deviation becomes less than this value, then $\sigma$-clipping will halt, see *note Sigma clipping::. ‘-g’ ‘--sigclipnum’ (‘=INT’) The number of iterations for the case where the $\sigma$-clipping iteration stops after a certain number of runs. ---------- Footnotes ---------- (1) If the ‘-q’ option is not called then all programs will operate in verbose mode, see *note Common options::.  File: gnuastro.info, Node: NoiseChisel, Next: MakeCatalog, Prev: ImageStatistics, Up: Image analysis 7.2 NoiseChisel =============== Once raw data have gone through the initial reduction process (through the programs in *note Image manipulation::). We are ready to derive scientific results out of them. Unfortunately in most cases, the scientifically interesting targets are deeply drowned in a sea of noise. NoiseChisel is Gnuastro’s tool to detect signal in noise. In fact, NoiseChisel was the motivation behind creating Gnuastro and has a journal article devoted to its techniques: arXiv:1505.01664 (http://arxiv.org/abs/1505.01664), published in 2015 by the Astrophysical Journal Supplement Series 220. Following the explanations for the options in *note NoiseChisel options:: should provide a relatively good idea of how NoiseChisel works, but it is recommended to see the paper since it does a very thorough job at explaining the concepts and methods of NoiseChisel with abundant demonstrations for each step. However, the paper cannot undergo any further updates, but NoiseChisel will evolve: better algorithms or steps will be found, thus options will be added or removed. So this section is the definitive guide. Please follow the ‘NEWS’ file with each release for such updates. Detection is the process of separating signal from noise. In other words, after detection is complete, one set of data elements (pixels in an image) will be distinguished as signal and another set of the data elements will be noise. Segmentation is the process of labeling the detected pixels into possibly multiple components (objects). For example when two galaxies lie sufficiently close to each other to be detected as one object. NoiseChisel was the first software to make use of a noise-based concept to detection and segmentation. In this method, instead of emphasizing on the signal and trying to guess the properties of the to-be-detected targets prior to detection (for example assuming that it is an ellipse), the emphasis is put on the noise in the image and it imposes statistically negligible requirements on the signal. The name of NoiseChisel is derived from the first thing it does after thresholding the image: to erode it. In mathematical morphology, erosion on pixels can be pictured as carving off boundary pixels. So what NoiseChisel does is similar to what a wood chisel or stone chisel do. It is just not a hardware but software. * Menu: * Invoking astnoisechisel:: Options and arguments for NoiseChisel.  File: gnuastro.info, Node: Invoking astnoisechisel, Prev: NoiseChisel, Up: NoiseChisel 7.2.1 Invoking NoiseChisel -------------------------- NoiseChisel will detect signal in noise. The executable name is ‘astnoisechisel’ with the following general template $ astnoisechisel [OPTION ...] InputImage.fits One line examples: $ astnoisechisel input.fits $ astnoisechisel --nch1=4 --lmesh=256 input.fits $ astnoisechisel field.fits --mask=badpixels.fits --mhdu=1 If NoiseChisel is to do processing, an input image should be provided with the recognized extensions as input data, see *note Arguments::. The options that are shared by all Gnuastro programs can be seen in *note Common options::. In order to ignore some pixels during the analysis, you can specify a mask image, see *note Mask image:: for an explanation and the relevant options. A masked pixel is completely ignored. A convolution kernel can also be optionally given. If a value (file name) is given to ‘--kernel’ on the command-line or in a configuration file (see *note Configuration files::), then that file will be used to convolve the image prior to thresholding. Otherwise a default kernel will be used. The default kernel is a 2D Gaussian with a FWHM of 2 pixels truncated at 5 times the FWHM. See Section 3.1.1 of Akhlaghi and Ichikawa (2015) to learn why this particular kernel was chosen as default. See *note Convolution kernel:: for kernel related options. NoiseChisel uses a mesh grid to tile the image. This enables it to deal with possible gradients, see *note Tiling an image::. The mesh grid options are common to all the programs using it, and are listed in *note Mesh grid options::. In particular, NoiseChisel uses two mesh grids: a large and a small one. The sizes of the meshs in each grid can be specified with the following two options (the ‘--meshsize’ option is not recognized by NoiseChisel). The rest of the options explained in *note Mesh grid options:: apply to both grids. ‘-s’ ‘--smeshsize’ Similar to ‘--meshsize’ in *note Mesh grid options::, but for the smaller mesh grid, which is most dependent on the gradients in the image. ‘-l’ ‘--lmeshsize’ Similar to ‘--meshsize’ in *note Mesh grid options::, but for the larger mesh grid, used for detection and segmentation Signal to noise ratio analysis. Please run NoiseChisel with the ‘--help’ option to list all the recognized options with a short explanation, irrespective of which part of the Gnuastro book they are fully explained in, see *note Getting help::. * Menu: * NoiseChisel options:: The options specific to NoiseChisel. * NoiseChisel output:: NoiseChisel’s output. Why no catalog?  File: gnuastro.info, Node: NoiseChisel options, Next: NoiseChisel output, Prev: Invoking astnoisechisel, Up: Invoking astnoisechisel 7.2.1.1 NoiseChisel options ........................... The options particular to NoiseChisel are listed below. They are classified by context and also sorted in the same order that the operations are done on the image. See Akhlaghi and Ichikawa (2015) for a very complete, detailed and illustrated explanation of each step. Reading through the option explanations should be enough to obtain a general idea of how NoiseChisel works. Before the procedures explained by these options begin, the image is convolved with a kernel. The first group of options listed below are those that apply to both the detection and the segmentation processes. ‘-E’ ‘--skysubtracted’ If this option is called, it is assumed that the image has already been sky subtracted once. Knowing if the sky has already been subtracted once or not is very important in estimating the Signal to noise ratio of the detections and clumps. In short an extra $\sigma_{sky}^2$ must be added in the error (noise or denominator in the Signal to noise ratio) for every flux value that is present in the calculation. This can be interpreted as the error in measuring that sky value when it was subtracted by any other program. See Section 3.3 in Akhlaghi and Ichikawa (2015) for a complete explanation. ‘-B’ ‘--minbfrac’ (‘=FLT’) Minimum fraction (value between 0 and 1) of blank (undetected) area in a mesh for it to be considered in measuring the following properties. • Measuring the Signal to noise ratio of false detections during the false detection removal. • Measuring the sky value (average of undetected pixels). Both before the removal of false detections and after it. • Clump Signal to noise ratio in the blank regions. Because of the PSF, astronomical objects, other than cosmic rays, never have a clear cutoff and commonly sink into the noise very slowly. Even below the very low thresholds used by NoiseChisel. So when a large fraction of the area of one mesh is covered by detections, it is very probable that their faint wings are present in the undetected regions. Therefore, to get an accurate measurement of the above parameters over the full mesh grid, meshs that harbor too many detected regions should be excluded. ‘-F’ ‘--minnumfalse’ (‘=INT’) The minimum number of ‘psudo-detections’ (in identifying false detections) or clumps (in identifying false clumps) in each large mesh grid. If their number is less than this value, this mesh will be left blank and filled during mesh interpolation, see *note Grid interpolation and smoothing::. The Signal to noise ratio of false detections and clumps in each mesh is found using the quantile of the Signal to noise ratio distribution of the psudo-detections and clumps over the undetected pixels in each mesh. If the number of Signal to noise ratio measurements in each mesh is not enough, the quantile will not be accurate. For example if you set ‘--detquant=0.99’ (or the top 1 percent), then it is best to have at least 100 Signal to noise ratio measurements. Detection is the process of separating the pixels in the image into two groups: 1) Signal and 2) Noise. Through the parameters below, you can customize the detection process in NoiseChisel. ‘-t’ ‘--qthresh’ (‘=FLT’) The quantile threshold to apply to the convolved image. The detection process begins with applying a quantile threshold to each of the small mesh grid elements, see *note Tiling an image::. The quantile is only calculated for those meshs that don’t have any significant signal within them, see *note Quantifying signal in a mesh::. The quantile value is a floating point value between 0 and 1. Assume that we have sorted the $N$ data elements of a distribution (the pixels in each mesh on the convolved image). The quantile ($q$) of this distribution is the value of the element with an index of (the nearest integer to) $q\times{N}$ in the sorted data set. After thresholding is complete, we will have a binary (two valued) image. The pixels above the threshold are known as foreground pixels (have a value of 1) while those which lie below the threshold are known as background (have a value of 0). ‘--checkthreshold’ Check the quantile threshold values on the mesh grid. A file suffixed with ‘_thresh.fits’ will be created, see *note Checking grid values::. ‘-e’ ‘--erode’ (‘=INT’) The number of erosions to apply to the binary thresholded image. Erosion is simply the process of flipping (from 1 to 0) any of the foreground pixels that neighbor a background pixel. In a 2D image, there are two kinds of neighbors, 4-connected and 8-connected neighbors. You can specify which type of neighbors should be used for erosion with the ‘--erodengb’ option, see below. Erosion has the effect of shrinking the foreground pixels. To put it another way, it expands the holes. This is a founding principle in NoiseChisel: it exploits the fact that with very low thresholds, the holes in the very low surface brightness regions of an image will be smaller than regions that have no signal. Therefore by expanding those holes, we are able to separate the regions harboring signal. ‘--erodengb’ (‘=4or8’) The type of neighborhood (structuring element) used in erosion, see ‘--erode’ for an explanation on erosion. In 4-connectivity, the neighbors of a pixel are defined as the four pixels on the top, bottom, right and left of a pixel that share an edge with it. The 8-connected neighbors on the other hand include the 4-connected neighbors along with the other 4 pixels that share a corner with this pixel. See Figure 6 (a) and (b) in Akhlaghi and Ichikawa (2015) for a demonstration. ‘--noerodequant’ Pure erosion is going to carve off sharp and small objects completely out of the detected regions. This option can be used to avoid missing such sharp and small objects (which have significant pixels, but not over a large area). All pixels with a value larger than the significance level specified by this option will not be eroded during the erosion step above. However, they will undergo the erosion and dilation of the opening step below. Like the ‘--qthresh’ option, the significance level is determined using the quantile (a value between 0 and 1). Just as a reminder, in the normal distribution, $1\sigma$, $1.5\sigma$, and $2\sigma$ are approximately on the 0.84, 0.93, and 0.98 quantiles. ‘-p’ ‘--opening’ (‘=INT’) Depth of opening to be applied to the eroded binary image. Opening is a composite operation. When opening a binary image with a depth of $n$, $n$ erosions (explained in ‘--erode’) are followed by $n$ dilations. Simply put, dilation is the inverse of erosion. When dilating an image any background pixel is flipped (from 0 to 1) to become a foreground pixel. Dilation has the effect of fattening the foreground. Note that in NoiseChisel, the erosion which is part of opening is independent of the initial erosion that is done on the thresholded image (explained in ‘--erode’). The structuring element for the opening can be specified with the ‘--openingngb’ option. Opening has the effect of removing the thin foreground connections (mostly noise) between separate foreground ‘islands’ (detections) thereby completely isolating them. Once opening is complete, we have _initial_ detections. ‘--openingngb’ (‘=4or8’) The structuring element used for opening, see ‘--erodengb’ for more information about a structuring element. ‘-u’ ‘--sigclumpmultip’ (‘=FLT’) The multiple of the standard deviation during $\sigma$-clipping. NoiseChisel uses $\sigma$-clipping to remove the effect of cosmic rays when calculating the average and standard deviation of the undetected regions. Since cosmic rays have sharp boundaries and are usually small, the erosion and opening might put them within the undetected pixels. Although they might cover a very small number of pixels, they usually have very large flux values which can easily bias the average and standard deviation measured on a mesh. Their effect can easily be removed by $\sigma$-clipping, see *note Sigma clipping::. NoiseChisel uses the convergence of the value of the standard deviation as the criteria to stop the $\sigma$-clipping iteration. ‘-r’ ‘--sigcliptolerance’ (‘=FLT’) The tolerance level to stop $\sigma$-clipping. The iteration is stopped when $(\sigma_{old}-\sigma_{new})/\sigma_{new}$ becomes smaller than the value given to this option. Note that $\sigma_{old}$ will always be larger than $\sigma_{new}$. Only statistical scatter (error) can cause it to be smaller, in which case they can be considered to be approximately equal. ‘--checkdetectionsky’ Check the initial approximation of the sky value and its standard deviation in a FITS file ending with ‘_detsky.fits’. See *note Checking grid values:: for more information. If ‘--meshbasedcheck’ is not called, then the first extension will be the the binary image with initial detections labeled one and background labeled zero. The mesh values will be in the subsequent extensions. ‘-R’ ‘--dthresh’ (‘=FLT’) The detection threshold: a multiple of the initial sky standard deviation added with the initial sky approximation. This flux threshold is applied to the initially undetected regions on the unconvolved image. The background pixels that are completely engulfed in a 4-connected foreground region are converted to background (holes are filled) and one opening (depth of 1) is applied over both the initially detected and undetected regions. The Signal to noise ratio of the resulting ‘psudo-detections’ are used to identify true vs. false detections. See Section 3.1.5 and Figure 7 in Akhlaghi and Ichikawa (2015) for a very complete explanation. ‘-i’ ‘--detsnminarea’ (‘=INT’) The minimum area to calculate the Signal to noise ratio on the psudo-detections of both the initially detected and undetected regions. When the area in a psudo-detection is too small, the Signal to noise ratio measurements will not be accurate and their distribution will be heavily skewed to the positive. So it is best to ignore any psudo-detection that is smaller than this area. Use ‘--detsnhistnbins’ to check if this value is reasonable or not. ‘--detsnhistnbins’ (‘=INT’) If not equal to zero, a histogram of the Signal to noise ratios of the psudo-detections will be stored in a text file ending with ‘_detsn.txt’. The number of bins in this histogram is specified by the value given to this option. This is good for inspecting the best possible value to ‘--detsnminarea’. An empirical way to estimate the best ‘--detsnminarea’ value for your data set is that the histogram have a sharp drop towards the higher S/Ns. In other words, when there is a prominent peak in the histogram and the last few bins have less than 10 (an arbitrary number, meaning very few!) pseudo-detections. When the minimum area is too large or too small, the slope of the histogram in the higher S/N bins will not be to sharp with the very high S/N bins having a large number of objects and the peak being less significant. A good minimum area will result in the last bins having very few pseudo-detections. ‘-c’ ‘--detquant’ (‘=FLT’) The quantile of the Signal to noise ratio distribution of the psudo-detections in each mesh to use for filling the large mesh grid. Note that this is only calculated for the large mesh grids that satisfy the minimum fraction of undetected pixels (value of ‘--minbfrac’) and minimum number of psudo-detections (value of ‘--minnumfalse’). ‘-I’ ‘--dilate’ (‘=INT’) Number of times to dilate the final true detections. See the explanations in ‘--opening’ for more information on dilation. The structuring element for this final dilation is fixed to an 8-connected neighborhood. This is because astronomical objects, except cosmic rays, never have a clear cutoff, so all the 8-pixels connected to the border pixels of a detection might harbor data. ‘--checkdetection’ Every step of the detection process will be added as an extension to a file with the suffix ‘_det.fits’. Going through each would just be a repeat of the explanations above and also of those in Akhlaghi and Ichikawa (2015). The extension label should be sufficient to recognize which step you are observing. Viewing all the steps can be the best guide in choosing the best set of parameters. Note that calling this function will significantly slow NoiseChisel. Normally the detection steps are done in parallel, but to show you each step individually, the parallel processing has to be halted and restarted multiple times. Below are some notes that might be useful in interpreting certain steps, beyond the paper. • Going from the first “Labeled†extension (for the background pseudo-detections, which shows the labeled pseudo-detections) to the next extension (“For S/Nâ€), with a relatively low ‘--dthresh’ value, you will notice that a lot of the large area pseudo-detections are removed and not used in calculating the S/N threshold. The main reason for this is that they overlap with possible detections. You can check by going to the next extension and seeing how there are detections there. The filled holes have been covering initial detections. If you have many such cases, it might be a good sign that your ‘--dthresh’ value is too low. ‘--checksky’ Check the final sky and its standard deviation values on the mesh grid. Similar to ‘--checkdetectionsky’. ‘--checkmaskdet’ Mask (set to NaN) the undetected pixels in one extension and the detected pixels in the next extension of a file ending with ‘_maskdet.fits’. Segmentation is the process of possibly breaking up a detection into multiple objects and clumps. In deep surveys segmentation becomes particularly important since galaxies might fall along the same line of sight or they might be merging. It is thus very important to be able separate the pixels within a detection if it is necessary. After segmentation, such a detected region will get different labels. In NoiseChisel, segmentation is done by first finding the ‘true’ clumps over a detection and then expanding those clumps to a certain flux limit. True clumps are found in a process very similar to the true detections explained above, see Akhlaghi and Ichikawa (2015) for more information. If the connections between the grown clumps are weaker than a given threshold, the grown clumps are considered to be separate objects. Otherwise, the are considered to be part of the same object. ‘--detectonly’ If this option is called, no segmentation will be done. The object labels extension in the output will simply be the detection (connected components) labels and the clumps image will be blank (see *note NoiseChisel output::). This option can result in faster processing when only the noise properties of the image are desired for a catalog using another image’s labels. A common case is when you want to measure colors or SEDs in several images. Let’s say you have images in two colors: A and B. For simplicity also assume that they are exactly on the same position in the sky with the same pixel scale. You choose to set A as a reference, so you run the full NoiseChisel on A. Then you run NoiseChisel on B with this option since you only need the noise properties of B (for the signal to noise column in its catalog). You can then run MakeCatalog on A normally, see *note MakeCatalog::. To run MakeCatalog on B, you simply set the object and clump labels images to those that NoiseChisel produced for A, see *note Invoking astmkcatalog::. ‘-m’ ‘--segsnminarea’ (‘=INT’) The minimum area which a clump in the undetected regions should have in order to be considered in the clump Signal to noise ratio measurement. If this size is set to a small value, the Signal to noise ratio of false clumps will not be accurately found. Note that this has to be larger than the value to ‘--detsnminarea’. Because the clumps are found on the convolved (smoothed) image while the psudo-detections are found on the input image. Use ‘--clumpsnhistnbins’ to check if this value is reasonable or not. ‘--clumpsnhistnbins’ (‘=INT’) Similar to ‘--detsnhistnbins’ (see there for more explanations), but for the distribution of the S/N of clumps over the undetected regions. The relevant parameter to check here is be ‘--segsnminarea’. ‘-g’ ‘--segquant’ (‘=FLT’) The quantile of the noise clump Signal to noise ratio distribution. This value is used to identify true clumps over the detected regions. ‘-v’ ‘--keepmaxnearriver’ Keep a clump whose maximum flux is 8-connected to a river pixel. By default such clumps over detections are considered to be noise and are removed irrespective of their brightness (see *note Flux Brightness and magnitude::). Over large profiles, that sink into the noise very slowly, noise can cause part of the profile (which was flat without noise) to become a very large and with a very high Signal to noise ratio. In such cases, the pixel with the maximum flux in the clump will be immediately touching a river pixel. ‘-G’ ‘--gthresh’ (‘=FLT’) Threshold (multiple of the sky standard deviation added with the sky) to stop growing true clumps. Once true clumps are found, they are set as the basis to segment the detected region. They are grown until the threshold specified by this option. ‘--grownclumps’ In the output (see *note NoiseChisel output::) store the grown clumps (or full detected region if only one clump was present in that detection). By default the original clumps are stored as the third extension of the output, if this option is called, it is replaced with the grown clump labels. ‘-y’ ‘--minriverlength’ (‘=INT’) The minimum length of a river between two grown clumps for it to be considered in Signal to noise ratio estimations. Similar to ‘--segsnminarea’ and ‘--detsnminarea’, if the length of the river is too short, the Signal to noise ratio can be noisy and unreliable. Any existing rivers shorter than this length will be considered as non-existent, independent of their Signal to noise ratio. Since the clumps are grown on the input image, this value should best be similar to the value of ‘--detsnminarea’. Recall that the clumps were defined on the convolved image so ‘--segsnminarea’ was larger than ‘--detsnminarea’. ‘-O’ ‘--objbordersn’ (‘=FLT’) The maximum Signal to noise ratio of the rivers between two grown clumps in order to consider them as separate ‘objects’. If the Signal to noise ratio of the river between two grown clumps is larger than this value, they are defined to be part of one ‘object’. Note that the physical reality of these ‘objects’ can never be established with one image, or even multiple images from one broad-band filter. Any method we devise to define ‘object’s over a detected region is ultimately subjective. Two very distant galaxies or satellites in one halo might lie in the same line of sight and be detected as clumps on one detection. On the other hand, the connection (through a spiral arm or tidal tail for example) between two parts of one galaxy might have such a low surface brightness that they are broken up into multiple detections or objects. In fact if you have noticed, exactly for this purpose, this is the only Signal to noise ratio that the user gives into NoiseChisel. The ‘true’ detections and clumps can be objectively identified from the noise characteristics of the image, so you don’t have to give any hand input Signal to noise ratio. ‘--checksegmentation’ A file with the suffix ‘_seg.fits’ will be created. This file keeps all the relevant steps in finding true clumps and segmenting the detections in various extensions. Having read the paper or the steps above, the extension name should be enough to understand which step each extension is showing. Examining this file can be an excellent guide in choosing the best set of parameters. Note that calling this function will significantly slow NoiseChisel.  File: gnuastro.info, Node: NoiseChisel output, Prev: NoiseChisel options, Up: Invoking astnoisechisel 7.2.1.2 NoiseChisel output .......................... The default name and directory of the outputs are explained in *note Automatic output::. NoiseChisel’s default output (when none of the options starting with ‘--check’ or the ‘--output’ option are called) is one file ending with ‘_labeled.fits’. This file has the extensions listed below: 1. A copy of the input image, a copy is placed here for the following reasons: • By flipping through the extensions, a user can check how accurate the detection and segmentation process was. • All the inputs to MakeCatalog (see *note MakeCatalog::) are included in this one file which makes the running of MakeCatalog after NoiseChisel very easy. • All masked pixels given to NoiseChisel will have a value of NaN in this image. So if you decide to run MakeCatalog after NoiseChisel, there is no more need to feed the mask image to MakeCatalog too. 2. The object labels. Each pixel in the input image is given a label in this extension, the labels start from one. The total number of labels is stored as the value to the ‘NOBJS’ keyword in the header of this extension. It is also printed in verbose mode. 3. The clump labels. All the pixels in the input image that belong to a true clump are given a positive label in this extension. The detected regions that were not a clump are given a negative value to clearly identify the noise from the detections. The total number of clumps in this image is stored in the ‘NCLUMPS’ keyword of this extension and printed in verbose output. If the ‘--grownclumps’ option is called, or a value of ‘1’ is given to it in any of the configuration files, then instead of the original clump regions, the grown clumps will be stored in this extension. Note that if there is only one clump (or no clumps) over a detected region, then the whole detected region is given a label of 1. 4. The final sky value on each pixel. See *note Sky value:: for a complete explanation. See *note Grid interpolation and smoothing:: for an explanation on the boxy appearance of this image. 5. Similar to the previous mesh but for the standard deviation on each pixel.  File: gnuastro.info, Node: MakeCatalog, Prev: NoiseChisel, Up: Image analysis 7.3 MakeCatalog =============== Detecting and segmenting signal over an image results in labeled images where each pixel is labeled with the ID (an integer) that is specified by the detector program. But this labeled image by its self can hardly be of any scientific use. The job of MakeCatalog is to combine the input image, the noise properties and the labels of pixels into a catalog (a text file table) which can easily be used for high-level scientific interpretations. NoiseChisel (Gnuastro’s signal detection tool, see *note NoiseChisel::) does not produce any catalog of the detected objects by its self. Only a labeled FITS image is output, see *note NoiseChisel output::. The output of NoiseChisel can be directly fed into MakeCatalog to generate the catalog. Some of the reasons for making the catalog in a separate program(1) are listed below: • Complexity: Adding in a catalog functionality to the detector program will add several more steps (and options) to its processing that can equally well be done outside of it. This makes following the code harder for a curious reader and also potentially adds bugs. Another advantage of less complexity is when the parameter you want to measure over one profile is not provided by the developers of MakeCatalog. You can simply open this tiny little program and add your desired calculation easily. In *note Adding new columns to MakeCatalog::, we have explained all the necessary steps to add a new column to MakeCatalog. However, if making a catalog was part of NoiseChisel, it would require a lot of energy to understand all the steps in order to add desired parameter. • Low level nature of Gnuastro: Making catalogs is a separate process from labeling (detecting and segmenting) the pixels. A user might want to do certain operations on the labeled regions before creating a catalog for them. Another user might want the properties of the same pixels in another image (possibly from another broadband filter) for measuring the colors or SEDs for example. Here is an example of doing both: suppose you have images in various broad band filters at various resolutions and orientations. The image of one color will thus not lie exactly on another or even be in the same scale. However, it is imperative that the same pixels be used in measuring the colors of galaxies. Therefore NoiseChisel can be run on the reference image and ImageWarp (*note ImageWarp::) can be applied to the labeled images to find the pixels to use in the other image. Then MakeCatalog can generate the final catalog for both targets. It is currently customary to warp the images to the same pixel grid, however, this is very harmful for the data and creates correlated noise. It is much more accurate to do the transformations on the labeled image. * Menu: * Quantifying data limits:: For comparing different catalogs. * Measuring elliptical parameters:: Estimating elliptical parameters. * Invoking astmkcatalog:: Options and arguments to MakeCatalog. * Adding new columns to MakeCatalog:: How to add new columns. ---------- Footnotes ---------- (1) Most existing software that do object detection also output a catalog, so this is not a common practice.  File: gnuastro.info, Node: Quantifying data limits, Next: Measuring elliptical parameters, Prev: MakeCatalog, Up: MakeCatalog 7.3.1 Quantifying data limits ----------------------------- Different datasets (images in the case of MakeCatalog) have different noise properties and different detection methods (or one method with a different set of parameters) will have different abilities to detect or measure certain kinds of objects in an image. Therefore it is very important to quantify our ability to detect and measure signal in noise. In this section we discuss these limits that are very important in any analysis. In astronomy, it is common to use the magnitude (a unit-less scale) and physical units, see *note Flux Brightness and magnitude::. Therefore all the measured discussed here are commonly defined in units of magnitudes. Depth As we make more observations on one region of the sky and add the images over each other, we are able to decrease the standard deviation of the noise in each pixel(1). Qualitatively, this decrease manifests its self by making fainter (per pixel) parts of the objects in the image more visible. Quantitatively, it increases the Signal to noise ratio, since the signal is fixed but the noise is decreased. It is very important to have in mind that here, noise is defined per pixel (or in the units of our data measurement), not per object. You can think of the noise as muddy water that is completely covering a flat ground(2) with some regions higher than the others(3) in it. In this analogy, height is brightness. Let’s assume that in your first observation the muddy water has just been stirred and you can’t see anything through it. As you wait and make more observations, the mud settles down and the _depth_ of the transparent water increases as you wait. The summits of hills begin to appear. As the depth of clear water increases, the parts of the hills with lower heights (less surface brightness) can be seen more clearly. The outputs of NoiseChisel include the Sky standard deviation ($\sigma$) on every group of pixels (a mesh) that were calculated from the undetected pixels in that mesh, see *note Tiling an image:: and *note NoiseChisel output::. Let’s take $\sigma_m$ as the median $\sigma$ over the successful meshes in the image (prior to interpolation or smoothing, see *note Grid interpolation and smoothing::). On different instruments pixels have different physical sizes (for example in micro-meters, or spatial angle over the sky), nevertheless, a pixel is our unit of data collection. In other words, while quantifying the noise, the physical or projected size of the pixels is irrelevant. We thus define the _depth_ of each data-set (or image) as the magnitude of $\sigma_m$. As an example, the XDF survey covers part of the sky that the Hubble space telescope has observed the most (for 85 orbits) and is consequently very small ($\sim4$ arcmin$^2$). On the other hand, the CANDELS survey, is one of the widest multi-color surveys covering several fields (about 720 arcmin$^2$) but its deepest fields have only 9 orbits observation. The depth of the XDF and CANDELS-deep surveys in the near infrared WFC3/F160W filter are respectively 34.40 and 32.45 magnitudes. In a single orbit image, this same field has a depth of 31.32. Recall that a larger magnitude corresponds to less brightness, see *note Flux Brightness and magnitude::. Upper limit magnitude Due to the noisy nature of data, it is possible to get arbitrarily low values for a faint object’s brightness (or arbitrarily high magnitudes). Given the scatter caused by the noise, such small values are meaningless: another similar depth observation will give a radically different value. This problem is most common when you use one image/filter to generate target labels (which specify which pixels belong to which object, see *note NoiseChisel output:: and *note MakeCatalog::) and another image/filter to generate a catalog for measuring colors. The object might not be visible in the filter used for the latter image, or the image _depth_ (see above) might be much shallower. So you will get unreasonably faint magnitudes. For example when the depth of the image is 32 magnitudes, a measurement that gives a magnitude of 36 for a $\sim100$ pixel object is clearly unreliable. In another similar depth image, we might measure a magnitude of 30 for it, and yet another might give 33. Furthermore, due to the noise scatter so close to the depth of the data-set, the total brightness might actually get measured as a negative value, so no magnitude can be defined (recall that a magnitude is a base-10 logarithm). Using such unreliable measurements will directly affect our analysis, so we must not use them. However, all is not lost! Given our limited depth, there is one thing we can deduce about the object’s magnitude: we can say that if something actually exists here (possibly buried deep under the noise), it must have a magnitude that is fainter than an _upper limit magnitude_. To find this upper limit magnitude, we place the object’s footprint (segmentation map) over random parts of the image where there are no detections, so we only have pure (possibly correlated) noise and undetected objects. Doing this a large number of times will give us a distribution of brightness values. The standard deviation ($\sigma$) of that distribution can be used to quantify the upper limit magnitude. Traditionally, faint/small object photometry was done using fixed circular apertures (for example with a diameter of $N$ arc-seconds). In this way, the upper limit was like the depth discussed above: one value for the whole image. But with the much more advanced hardware and software of today, we can make customized segmentation maps for each object. The number of pixels (are of the object) used directly affects the final distribution and thus magnitude. Also the image correlated noise might actually create certain patters, so the shape of the object can also affect the result. So in MakeCatalog, the upper limit magnitude is found for each object in the image separately. Not one value for the whole image. Completeness limit As the surface brightness of the objects decreases, the ability to detect them will also decrease. An important statistic is thus the fraction of objects of similar morphology and brightness that will be identified with our detection algorithm/parameters in the given image. This fraction is known as completeness. For brighter objects, completeness is 1: all bright objects that might exist over the image will be detected. However, as we go to lower surface brightness objects, we fail to detect some and gradually we are not able to detect anything any more. For a given profile, the magnitude where the completeness drops below a certain level usually above $90\%$ is known as the completeness limit. Another important parameter in measuring completeness is purity: the fraction of true detections to all true detections. In effect purity is the measure of contamination by false detections: the higher the purity, the lower the contamination. Completeness and purity are anti-correlated: if we can allow a large number of false detections (that we might be able to remove by other means), we can significantly increase the completeness limit. One traditional way to measure the completeness and purity of a given sample is by embedding mock profiles in regions of the image with no detection. However in such a study we must be really careful to choose model profiles as similar to the target of interest as possible. ---------- Footnotes ---------- (1) This is true for any noisy data, not just astronomical images (2) The ground is the sky value in this analogy, see *note Sky value::. Note that this analogy only holds for a flat sky value across the surface of the image or ground. (3) The peaks are (parts of) astronomical objects in this analogy.  File: gnuastro.info, Node: Measuring elliptical parameters, Next: Invoking astmkcatalog, Prev: Quantifying data limits, Up: MakeCatalog 7.3.2 Measuring elliptical parameters ------------------------------------- One of the most important class of parameters that are important for astronomical image analysis is the shape or morphology of the objects. In the case of galaxies (with a very rich variety of morphologies) studying the morphology of the detected objects is its self a is very complicated research subject which is a very active field of research now. So in this section, we will just discuss how the most basic morphological parameters are estimated: the elliptical parameters for a set of labeled pixels (that will be studied together and define our object of interest). These are: the major axis, the minor axis and the position angle along with the central position of the profile. The derivations below follow the SExtractor manual derivations but include more explanations. Let’s begin with one dimension for simplicity: Assume we have a set of $N$ values (brightness for example) $B_i$, each at position $x_i$. The simplest parameter we can define is the geometric center of the object ($x_g$) (ignoring the brightness values): $x_g=(\sum_ix_i)/N$. _Moments_ are defined to incorporate both the value (brightness) and position of the data. The first moment can be written as: $$\overline{x}={\sum_iB_ix_i \over \sum_iB_i}$$ This is essentially the weighted (by $B_i$) average position. The geometric center ($x_g$, defined above) is a special case of this with all $B_i=1$. The second moment is essentially the variance of the distributions: $$\overline{x^2}\equiv{\sum_i(B_ix_i-\overline{x})^2 \over \sum_iB_i} ={\sum_iB_i^2x_i^2 \over \sum_iB_i} - 2\overline{x}{\sum_iB_ix_i\over\sum_iB_i} + \overline{x}^2 ={\sum_iB_i^2x_i^2 \over \sum_iB_i} - \overline{x}^2$$ The last step was done from the definition of $\overline{x}$. So the square root of $\overline{x^2}$ is the positional standard deviation (along the one-dimensional) of this particular brightness distribution ($B_i$). Crudely (or qualitatively), you can think of its square root as the distance (from $\overline{x}$) which contains a specific amount of the flux (depending on the $B_i$ distribution). Similar to the first moment, the geometric second moment can be found by setting all $B_i=1$. So while the first moment quantified the position of the brightness distribution, the second moment quantifies how that brightness is dispersed about the first moment. In other words, it quantifies how “sharp†the object’s image is. Before continuing to two dimensions and the derivation of the elliptical parameters we will pause for an implementation technicality. You can ignore this paragraph if you don’t want to implement these concepts. The basic definition (first fraction for $\overline{x^2}$) can be used without any major problem. However, using this fraction requires two runs over the data: one run to specify $\overline{x}$ and one run for $\overline{x^2}$, this can be slow. However, using the last fraction above, we can estimate both the first and second moments in one run (since the $-\overline{x}^2$ term can easily be added later). Using the last form creates a major technical issue however: due to the floating point accuracy. Suppose the object is located between pixels 10000 and 10020. While the object pixels are only distributed over 20 pixels (with a standard deviation $<20$), the mean has a value of $\sim10000$. The $\sum_iB_i^2x_i^2$ will go to very very large values while the individual pixel differences will be much smaller, this will lower the accuracy of our calculation due to the limited accuracy of floating point operations. Since the variance only depends on the distance of each point from the mean, and for a constant/arbitrary $K$, $\overline{x-K}=\overline{x}-K$, we can calculate the second order moment using: $$\overline{x^2}={\sum_iB_i^2(x_i-K)^2 \over \sum_iB_i} - (\overline{x}-K)^2$$ The closer $K$ is to $\overline{x}$, the better (the sums of squares will involve smaller numbers), as long as $K$ is within the object limits (in the example above: $10000\leq{K}\leq10020$), the floating point error induced in our calculation will be negligible. For the most simplest implementation, in order to find the second moments (variance) in each dimension, MakeCatalog takes $K$ to be the position of the first pixel that is assigned to the object under each dimension. Since $K$ is arbitrary and an implementation/technical detail, we will ignore it for the remainder of this discussion. In two dimensions, the mean and variances can be written as: $$\overline{x}={\sum_iB_ix_i\over B_i}, \quad \overline{x^2}={\sum_iB_i^2x_i^2 \over \sum_iB_i} - \overline{x}^2$$ $$\overline{y}={\sum_iB_iy_i\over B_i}, \quad \overline{y^2}={\sum_iB_i^2y_i^2 \over \sum_iB_i} - \overline{y}^2$$ $$\quad\quad\quad\quad\quad\quad\quad\quad\quad \overline{xy}={\sum_iB_i^2x_iy_i \over \sum_iB_i} - \overline{x}\times\overline{y}$$ If an elliptical profile’s major axis lies exactly along the $x$ axis, then $\overline{x^2}$ will be directly proportional with the major axis, $\overline{y^2}$ with its minor axis and $\overline{xy}=0$. However, in reality we are not that lucky and (assuming galaxies can be parametrized as an ellipse) the major axis of galaxies can be in any direction on the image (in fact this is one of the core principles behind weak-lensing by shear estimation). So the purpose of the remainder of this section is to define a strategy to measure the position angle and axis ratio of some randomly positioned ellipses in an image, using the raw second moments that we have calculated above in our image coordinates. Let’s assume we have rotated the galaxy by $\theta$, then the new second order moments can be written as: $$\overline{x_\theta^2} = \overline{x^2}\cos^2\theta + \overline{y^2}\sin^2\theta - 2\overline{xy}\cos\theta\sin\theta $$ $$\overline{y_\theta^2} = \overline{x^2}\sin^2\theta + \overline{y^2}\cos^2\theta + 2\overline{xy}\cos\theta\sin\theta$$ $$\overline{xy_\theta} = \overline{x^2}\cos\theta\sin\theta - \overline{y^2}\cos\theta\sin\theta + \overline{xy}(\cos^2\theta-\sin^2\theta)$$ We can now find the best $\theta$ ($\theta_0$) such that the major axis lies along the $x_\theta$ axis. This can be found by setting: $$\left.{\partial \overline{x_\theta^2} \over \partial \theta}\right|_{\theta_0}=0$$ Taking the derivative, we get: $$2\cos\theta_0\sin\theta_0(\overline{y^2}-\overline{x^2}) + 2(\cos^2\theta_0-\sin^2\theta_0)\overline{xy}=0$$ When $\overline{x^2}\neq\overline{y^2}$, we can write: $$\tan2\theta_0 = 2{\overline{xy} \over \overline{x^2}-\overline{y^2}}.$$ MakeCatalog uses the standard C math library’s ‘atan2’ function to estimate $\theta_0$, which we define as the position angle of the ellipse. To recall, this is the angle of the major axis of the ellipse with the $x$ axis. By definition, when the elliptical profile is rotated by $\theta_0$, then $\overline{xy_{\theta_0}}=0$, $\overline{x_{\theta_0}^2}$ will be the extent of the maximum variance and $\overline{y_{\theta_0}^2}$ the extent of the minimum variance (which are perpendicular for an ellipse). Replacing $\theta_0$ in the equations above for $\overline{x_\theta}$ and $\overline{y_\theta}$, we can get the semi-major ($A$) and semi-minor ($B$) lengths: $$A^2\equiv\overline{x_{\theta_0}^2}= {\overline{x^2} + \overline{y^2} \over 2} + \sqrt{\left({\overline{x^2}-\overline{y^2} \over 2}\right)^2 + \overline{xy}^2}$$ $$B^2\equiv\overline{y_{\theta_0}^2}= {\overline{x^2} + \overline{y^2} \over 2} - \sqrt{\left({\overline{x^2}-\overline{y^2} \over 2}\right)^2 + \overline{xy}^2}$$ So as a summary, it is important to remember that the units of $A$ and $B$ are in pixels (same as the standard deviation) and that they represent the spatial light distribution of the object in both image dimensions if the object could be approximated as an ellipse. When the object cannot be represented as an ellipse, this interpretation breaks down: $\overline{xy_{\theta_0}}\neq0$ and $\overline{y_{\theta_0}^2}$ will not be the direction of minimum variance.  File: gnuastro.info, Node: Invoking astmkcatalog, Next: Adding new columns to MakeCatalog, Prev: Measuring elliptical parameters, Up: MakeCatalog 7.3.3 Invoking MakeCatalog -------------------------- MakeCatalog will make a catalog from an input image and at least on labeled image. The executable name is ‘astmkcatalog’ with the following general template $ astmkcatalog [OPTION ...] InputImage.fits One line examples: $ astmkcatalog -mdri input.fits $ astmkcatalog --floatprecision=5 input.fits $ astmkcatalog --output=cat input_labeled.fits $ astmkcatalog --objlabs=K_labeled.fits --objhdu=1 \ --clumplabs=K_labeled.fits --clumphdu=2 i_band.fits If MakeCatalog is to do processing, an input image should be provided with the recognized extensions as input data, see *note Arguments::. Optionally a mask file can be specified to ignore some of the pixels in the image, see *note Mask image::. Note that if you generated the labeled image using NoiseChisel with a mask image as input, there is no more need to inform MakeCatalog of the mask image, see *note NoiseChisel output::. The options common to all Gnuastro programs are explained in *note Common options::. MakeCatalog needs 4 (or 5) images as input. These images can be separate extensions in one file (NoiseChisel’s default output), or each can have its own file and its own extension. The full 5 images are listed in *note NoiseChisel output::. However, the clump labels image is not mandatory (when no clump catalog is required, for example in aperture photometry). When inspecting the object labels image, MakeProfiles will look for a ‘WCLUMPS’ (short for with-clumps) header keyword. If that keyword is present and has a value of ‘yes’ (not case sensitive, so ‘Yes’, or ‘YES’ are also acceptable) then a clump image must also be provided and a clump catalog will be made. When ‘WCLUMPS’ isn’t present or has any other value, only an object catalog will be created and all clump related options will be ignored. For example, if you only need an object catalog from NoiseChisel’s output, you can use Header (see *note Header::) to modify or remove the ‘WCLUMPS’ keyword in the objects HDU, then run MakeCatalog on it. Another example can be aperture photometry: let’s assume you have made your labeled image (defining the apertures) with MakeProfiles. Clumps are not defined in this context, so besides the input and labeled image, you only need NoiseChisel’s Sky and Sky standard deviation images. Since MakeProfile’s output doesn’t contain the ‘WCLUMPS’ keyword, you just have to specify your labeled image with the ‘--objlabs’ option and also set its HDU and no clumps catalog will be created. Note that labeled images have to be an integer type. Therefore, when using MakeProfiles to define the apertures/labels, you can use ‘--type=long’ for example. When a clump catalog is also desired, two catalogs will be made: one for the objects (suffixed with ‘_o.txt’) and another for the clumps (suffixed with ‘_c.txt’). Therefore if any value is given to the ‘--output’ option, MakeCatalogs will replace these two suffixes with any existing suffix in the given value. If no output value is given, MakeCatalog will use the input name, see *note Automatic output::. When only building an object catalog, any suffix in the value to output will just be replaced with ‘.txt’. The first set of options specify the properties of the inputs. Other necessary input images are treated very much like a mask image, see *note Mask image::. If no name is specified for them, their HDU is checked and if that differs from the input HDU, then there is no need to specify a file name for them. The object and column label images or segmentation maps should not be of a floating point type (‘BITPIX’). ‘-O’ ‘--objlabs’ (‘=STR’) The file name of the object labels, if in the same file as input, it is not mandatory. ‘--objhdu’ (‘=STR’) The HDU of the object labels image, the header keyword ‘NOBJS’ must be present in this extension. The value to this keyword is used as the final number of objects and the number of rows in the output objects catalog. Only pixels with values above zero will be considered. ‘-c’ ‘--clumplabs’ (‘=STR’) Similar to ‘--objlabs’ but for the labels of the clumps. ‘--clumphdu’ (‘=STR’) Similar to ‘--objhdu’, but for the clumps. The ‘NCLUMPS’ keyword in this header specifies the number of recognized clumps. ‘-s’ ‘--skyfilename’ (‘=STR’) File name of an image keeping the Sky value for each pixel. ‘--skyhdu’ (‘=STR’) The HDU of the Sky value image. ‘-t’ ‘--stdfilename’ (‘=STR’) File name of image keeping the Sky value standard deviation for each pixel. ‘--stdhdu’ (‘=STR’) The HDU of the Sky value standard deviation image. ‘-z’ ‘--zeropoint’ (‘=FLT’) The zero point magnitude for the input image, see *note Flux Brightness and magnitude::. ‘-E’ ‘--skysubtracted’ If the image has already been sky subtracted by another program, then you need to notify MakeCatalog through this option. Note that this is only relevant when the Signal to noise ratio is to be calculated. ‘-T’ ‘--threshold’ (‘=FLT’) For all the columns, only consider pixels that are above a given relative threshold. Symbolizing the value of this option as $T$, the Sky for a pixel at $(i,j)$ with $\mu_{ij}$ and its Standard deviation with $\sigma_{ij}$, that pixel will only be used if its value ($B_{ij}$) satisfies this condition: $B_{ij}>\mu_{ij}+{T}\sigma_{ij}$. The only calculations that will not be affected are is the average river values (‘--riverave’), since they are used as a reference. A commented row will be added in the header of the output catalog that will print the given value, since this is a very important issue, it starts with ‘**IMPORTANT**’. NoiseChisel will detect very diffuse signal which is useful in most cases where the aggregate properties of the detections are desired, since there is signal there (with the desired certainty). However, in some cases, only the properties of the peaks of the objects/clumps are desired, for example in attempting to separate stars from galaxies, the peaks are the major target and the diffuse regions only act to complicate the separation. With this option, MakeCatalog will simply ignore any pixel below the relative threshold. This option is not mandatory, so if it isn’t given (after reading the command-line and all configuration files, see *note Configuration files::), MakeCatalog will still operate. However, if it has a value in any lower-level configuration file and you want to ignore that value for this particular run or in a higher-level configuration file, then set it to NaN, for example ‘--threshold=nan’. Gnuastro uses the C library’s ‘strtod’ function to read floats, which is not case-sensative in reading NaN values. But to be consistent, it is good practice to only use ‘nan’. Through the next group of options, you can customize the general output plain text catalog. The basic idea behind the options about the width and precision of the different types is the fact that some columns don’t need too much space, while some do. The width is the number of text columns given to data of each type in the output plain text catalog. The precision is the number of digits to show after the decimal point in floating point numbers. We have defined two types of floating point numbers here, one is for less accurate precision, like magnitude, while the other is used when more accuracy is necessary. A common example of the latter is right ascension and declination. These variables usually need to be printed with more than 6 point accuracy. Note that all the values are calculated and stored internally as double precision floating point numbers, the distinction made here is only for printing them. ‘--nsigmag’ (‘=FLT’) The magnitude of the value to this option multiplied by the maximum standard deviation over the objects or clumps is reported in the output catalog. This value is a per-pixel value, not per object and is not found over an area or aperture, like the common $5\sigma$ values that are commonly reported as a measure of depth. They are based on a certain area and are relics from the time of analog data collection and processing. Modern tools use digital imaging detectors and the area is that of a pixel. ‘--intwidth’ (‘=INT’) The width of printing the integer values. In MakeCatalog, all IDs, numbers (counters) and areas are considered to be an integer. ‘--floatwidth’ (‘=INT’) The width of a normal precision floating point column. Any column that is not designated in ‘--intwidth’ or ‘--accuwidth’ is considered to be a normal precision floating point. ‘--accuwidth’ (‘=INT’) The width columns to be printed with extra accuracy. In MakeCatalog the following columns are printed with extra accuracy: right ascension, declination, brightness, river pixel averages (see Akhlaghi and Ichikawa 2015 for the definition of river pixels), the sky and the sky standard deviation. ‘--floatprecision’ (‘=INT’) The number of digits to the right of the decimal point in normal floating point display. ‘--accuprecision’ (‘=INT’) The number of digits to the right of the decimal point in more accurate floating point display. The upper limit magnitude was discussed in *note Quantifying data limits::. Unlike other measured values/columns in MakeCatalog, the upper limit magnitude needs several defined parameters which are discussed here. All the upper limit magnitude specific options start with ‘up’ for upper limit, except for ‘--envseed’ that is also present in other programs and is general for any job requiring random number generation. One very important consideration in Gnuastro is reproducibility. Therefore, the values to all of these parameters along with others (like the random number generator type and seed) are also reported in the comments of the final catalog when the upper limit magnitude column is desired. One of those parameters is the number of threads used in this run of MakeCatalog. This might seem irrelevant. The job of sampling a large number of positions over the image is an “embarrasingly parallel†kind of problem which can greatly benefit from threads. For maximum efficiency, the objects in the catalog are divided between the threads and the random number generator is used independently on each thread. So even when the random number generator type and seed are identical, if the number of threads differ, you will get different results. Ofcourse, the difference is due to scatter and is statistically negligible, but it is not exactly reproducible (which is important in some contexts). ‘--upmask’ (‘=STR’) File name of mask image to use for upper-limit calculation. In some cases (especially when doing matched photometry), the object labels specified in the main input and mask image might not be adequate. In other words they do not necessarily have to cover _all_ detected objects: the user might have selected only a few of the objects in their labeled image. All the non-zero pixels of the image specified by this option (in the ‘--upmaskhdu’ extension) will be set as blank for the upper limit magnitude calculation. For example, when you are using labels from another image, you can give NoiseChisel’s objects image output for this image as the value to this option. In this way, you can be sure that regions with data do not harm your distribution. See *note Quantifying data limits:: for more on the upper limit magnitude. ‘--upmaskhdu’ (‘=STR’) The extension in the file specified by ‘--upmask’. ‘--upnum’ (‘=INT’) The number of random samples to take for all the objects. A larger value to this option will give a more accurate result (assymptotically), but it will also slow down the process. When a randomly positioned sample overlaps with a detected/masked pixel it is not counted and another random position is found until the object completely lies over an undetected region. So you can be sure that for each object, this many samples over undetected objects are made. See the upper limit magnitude discussion in *note Quantifying data limits:: for more. ‘--envseed’ Read the random number generator type and seed value from the environment (see *note Generating random numbers::). Random numbers are used in calculating the random positions of different samples of each object. ‘--upsclipmultip’ (‘=FLT’) The multiple of $\sigma$ to use in $\sigma$-clipping the final distribution (see *note Sigma clipping::). The images might have some artifacts or some regions with signal in the image might not have been removed correctly. If a random sampling falls over such regions, they can significantly bias the final standard deviation. To avoid the effect of such outliers, after the distribution is found, it is $\sigma$-clipped (by convergence). ‘--upsclipaccu’ (‘=FLT’) Relative difference between two successive $\sigma$ measurements to halt the $\sigma$-clipping process by convergence, see the explanations for ‘--upsclipmultip’ for more. ‘--upnsigma’ (‘=FLT’) The multiple of the standard deviation (or $\sigma$) used to measure the magnitude. Note that this is the final $\sigma$ produced after the $\sigma$-clipping. The final group of options particular to MakeCatalog are those that specify which columns should be displayed in the output catalogs. For each column there is an option, if it has been called on the command line or in any of the configuration files, it will included as a column in the output catalog. Some of the options apply to both objects and clumps and some are particular to only one of them. The latter cases are explicitly marked with [Objects] or [Clumps] to specify the catalog they will be placed in. The order of the columns in the output catalog is the inverse of the order their options are read in. For example see the following command(1): $ astmkcatalog --magnitude --dec --ra --id input.fits In this example, if no columns are specified in any of the configuration files (see *note Configuration files::), then the columns in the catalogs produced by this command will have the following order: ID, RA, Dec and Magnitude. Contrary to what it looks like, this is done to make life easier for the users. The configuration files can also keep any of the columns (so you don’t have to specify your desired columns every time). This inverse ordering thus comes from their precedence, see *note Configuration file precedence::. For example catalogs usually have at least an ID column and position columns (in the image and/or the world coordinate system). By reading the order of the columns in reverse you can have your fixed set of columns in your system wide configuration file and in any particular run, if you want some other information about objects or clumps, you can add those columns on the command-line. Through the user and current directory configuration files, you can also have custom catalogs in each of your working directories, without bothering to specify the columns every time you run MakeCatalog in those directories. ‘--i’ ‘--id’ The ID of the clump or object. ‘-j’ ‘hostobjid’ [Clumps] The ID of the object which hosts this clump. ‘-I’ ‘--idinhostobj’ [Clumps] The ID of this clump in its host object. ‘-C’ ‘--numclumps’ [Objects] The number of clumps in this object. ‘-a’ ‘--area’ The area (number of pixels) in any clump or object. ‘--clumpsarea’ [Objects] The total area of all the clumps in this object. ‘-x’ ‘--x’ The flux weighted center of all objects and clumps along the first FITS axis (horizontal when viewed in SAO ds9). The weight has to have a positive value (pixel value larger than the Sky value) to be meaningful! Specially when doing matched photometry, this might not happen: no pixel value might be above the Sky value. In such cases, where there was no pixel with a value larger than the Sky in the object or clump, the geometric center (ignoring pixel values, only their positions) over the object or clump is used instead of the flux weighted center (see ‘--geox’). ‘-y’ ‘--y’ The flux weighted center of all objects and clumps along the second FITS axis (vertical when viewed in SAO ds9). See ‘--x’. ‘--geox’ The geometric center of all objects and clumps along the first FITS axis axis. The geometric center is the average pixel positions irrespective of their pixel values. ‘--geoy’ The geometric center of all objects and clumps along the second FITS axis axis, see ‘--geox’. ‘--clumpsx’ [Objects] The flux weighted center of all the clumps in this object along the first FITS axis. See ‘--x’. ‘--clumpsy’ [Objects] The flux weighted center of all the clumps in this object along the second FITS axis. See ‘--x’. ‘--clumpsgeox’ [Objects] The geometric center of all the clumps in this object along the first FITS axis. See ‘--geox’. ‘--clumpsgeoy’ [Objects] The geometric center of all the clumps in this object along the second FITS axis. See ‘--geox’. ‘-r’ ‘--ra’ Flux weighted right ascension of all objects or clumps, see ‘--x’. ‘-d’ ‘--dec’ Flux weighted declination of all objects or clumps, see ‘--x’. ‘--geora’ Geometric center right ascension of all objects or clumps, see ‘--geox’. ‘--geodec’ Geometric center declination of all objects or clumps, see ‘--geox’. ‘--clumpsra’ [Objects] Flux weighted right ascension of all clumps in this object, see ‘--x’. ‘--clumpsdec’ [Objects] Flux weighted declination of all clumps in this object, see ‘--x’. ‘--clumpsgeora’ [Objects] Geometric center right ascension of all clumps in this object, see ‘--geox’. ‘--clumpsgeodec’ [Objects] Geometric center declination of all clumps in this object, see ‘--geox’. ‘-b’ ‘--brightness’ The brightness (sum of all pixel values), see *note Flux Brightness and magnitude::. For each clump in the clumps catalog, the ambient brightness (flux of river pixels around the clump multiplied by the area of the clump) is removed, see ‘--riverflux’. So the sum of clump brightnesses in the clump catalog will be smaller than the total clump brightness in the ‘--clumpbrightness’ column of the objects catalog. ‘--clumpbrightness’ [Objects] The total brightness of the clumps within an object. This is simply the sum of the pixels associated with clumps in the object. ‘--noriverbrightness’ [Clumps] The Sky (not river) subtracted clump brightness. By definition, for the clumps, the average brightness of the rivers surrounding it are subtracted from it for a first order accounting for contamination by neighbors. In cases where you will be calculating the flux brightness difference later (one example below) the contamination will be (mostly) removed at that stage, which is why this column was added. One example might be this: you want to know the change in the clump flux as a function of threshold (see ‘--threshold’). So you will make two catalogs (each having this column but with different thresholds) and then subtract the lower threshold catalog (higher brightness) from the higher threshold catalog (lower brightness). The effect is most visible when the rivers have a high average signal-to-noise ratio. The removed contribution from the pixels below the threshold will be less than the river pixels. Therefore the river-subtracted brightness (‘--brightness’) for the thresholded catalog for such clumps will be larger than the brightness with no threshold! ‘-m’ ‘--magnitude’ The magnitude of clumps or objects, see ‘--brightness’. ‘-e’ ‘--magnitudeerr’ The magnitude error of clumps or objects. The magnitude error is calculated from the signal-to-noise ratio (see ‘--sn’, abbreviated as $S$): $\Delta{M}=2.5/(S\times\ln{10})$. Note that until now this error assumes un-correlated pixel values and also does not include the error in estimating the aperture (or error in generating the labeled image). For now these factors have to be found by other means. Task 14124 (https://savannah.gnu.org/task/index.php?14124) has been defined for work on adding these sources of error too. ‘--clumpsmagnitude’ [Objects] The magnitude of all clumps in this object, see ‘--clumpbrightness’. ‘--upperlimitmag’ [Objects] The upper limit magnitude for this object. The object’s footprint is used over randomly positioned parts of the image that do not cover a detected object. The standard deviation of the final distribution is then the upper limit magnitude, see *note Quantifying data limits:: for a complete explanation. This is very important for the fainter objects in the image where the measured magnitudes are not reliable. ‘--riverave’ [Clumps] The average brightness of the river pixels around this clump. River pixels were defined in Akhlaghi and Ichikawa 2015. In short they are the pixels immediately outside of the clumps. This value is used internally to find the brightness (or magnitude) and signal to noise ratio of the clumps. It can generally also be used as a scale to gauge the base (ambient) flux surrounding the clump. In case there was no river pixels, then this column will have the value of the Sky under the clump. So note that this value is _not_ sky subtracted. ‘--rivernum’ [Clumps] The number of river pixels around this clump, see ‘--riverflux’. ‘-n’ ‘--sn’ The Signal to noise ratio (S/N) of all clumps or objects. See Akhlaghi and Ichikawa (2015) for the exact equations used. ‘--sky’ The sky flux (per pixel) value under this object or clump. This is actually the mean value of all the pixels in the sky image that lie on the same position as the object or clump. ‘--std’ The sky value standard deviation (per pixel) for this clump or object. Like ‘--sky’, this is the average of the values in the input sky standard deviation image pixels that lie over this object. ‘-A’ ‘--semimajor’ The pixel-value weighted semi-major axis of the profile (assuming it is an ellipse) in units of pixels. ‘-B’ ‘--semiminor’ The pixel-value weighted semi-minor axis of the profile (assuming it is an ellipse) in units of pixels. ‘-p’ ‘--positionangle’ The pixel-value weighted angle of the semi-major axis with the first FITS axis in degrees. ‘--geosemimajor’ The geometric (ignoring pixel values) semi-major axis of the profile, assuming it is an ellipse. ‘--geosemiminor’ The geometric (ignoring pixel values) semi-minor axis of the profile, assuming it is an ellipse. ‘--geopositionangle’ The geometric (ignoring pixel values) angle of the semi-major axis with the first FITS axis in degrees. ---------- Footnotes ---------- (1) This command is practically identical to the first command in the one-line examples, see *note Options:: for an explanation of the concatenation of the on/off options.  File: gnuastro.info, Node: Adding new columns to MakeCatalog, Prev: Invoking astmkcatalog, Up: MakeCatalog 7.3.4 Adding new columns to MakeCatalog --------------------------------------- The common development characteristics of MakeCatalog and other Gnuastro programs is explained in *note Developing::. This section might be more clearly understood after reading that chapter. MakeCatalog has been designed to allow easy addition of new columns, here we will give a fast over-view of the steps you need to take to define a new output column. After adding and testing your column, you are most welcome (and encouraged) to share it with us so we can add to the next release of Gnuastro for everyone else to also benefit from your efforts. MakeCatalog will first have two passes over the input pixels: in the first pass it will gather mainly object information and in the second run, it will mainly focus on the clumps, or any other measurement that needs an output from the first pass. These two passes are designed to be raw summations: no extra processing. This will allow parallel processing and simplicity/clarity. Once the passes are done, depending on the order of options that the user has defined the appropriate function will be called to add a processed column from the raw calculations to the output array (which will be printed). So if your new calculation, needs new raw information from the pixels, then you will need to also modify the respective ‘firstpass’ and ‘secondpass’ functions and define new information table columns in ‘main.h’. For all the steps below, it is easiest to just copy and paste an existing option and change the variables in each step. In all these different places, the options are sorted in the same order (same order as *note Invoking astmkcatalog::). This allows a particular column/option to be easily found in all steps. Therefore in adding your new option, be sure to keep it in the same relative place in the list in all the separate places (it doesn’t necessarily have to be in the end), and near conceptually similar options. ‘main.h’ The ‘objectcols’ and ‘clumpcols’ enumerated variables (‘enum’) define the labels for the separate information table columns (the raw pixel calculations). If your new calculation requires new raw columns, the add new macros for them. The ‘outcols’ enumerated variables define the recognized output columns. You will need to add a new name for your desired column here, then add a row for your new parameter in the ‘uiparams’ structure, the name should be the same as the one you used in ‘outcols’ (in small caps). ‘args.h’ This file specifies all the parameters for the GNU C library, Argp structure that is in charge of reading the user’s options. It is best that the option name be the same as the name you put in ‘outcols’ (in ‘main.h’), like the other options that are already defined. Define a new option in ‘argp_option’ (rows between the ‘{’ and ‘}’). The first is the name of the option, the second is its short option name (see *note Options::). The next two values should be ‘0’ and the last should be a short description of your option/column. For the second element is best to use a number (so no short option is defined for the user) which in Gnuastro is defined to be a number larger than 500. The range of used numbers (and short option names) are shown in the comment immediately above ‘argp_option’ structure, increase that number by one and use that number for your new option. Go down to the ‘parse_opt’ function and add a ‘case’ for your specific option (using the same number you specified above), then update the contents, based on the new macros you defined ‘main.h’. ‘ui.c’ In the ‘readconfig’ function, add an ‘else if’ for your option (easiest to just copy and paste, then update). In the ‘printvalues’ function’s ‘switch’ structure, add a ‘case’ for your option. Finally, in the ‘preparearrays’ function, add a ‘case’ for your new output column. Note that if the column is to be used for both objects and clumps, you need to set both ‘p->objcols’ and ‘p->clumpcols’. ‘mkcatalog.c’ If your procedure needs new raw calculations, add a new line to appropriate parts of the ‘firstpass’, and/or ‘secondpass’ functions, they should be clear and are fully commented. Then add a ‘case’ for your column in the ‘makeoutput’ function, here you will need to call a function (which should be defined in ‘columns.c’). ‘columns.c’ Define the function that will write your desired column in the output column using the raw input calculations here. There are a lot of functions in this file which you can use to model and they are commented, in short you have to specify a header (commented column), the units of your variable, the possible accuracy to print and finally the actual columns.  File: gnuastro.info, Node: Modeling and fittings, Next: High-level calculations, Prev: Image analysis, Up: Top 8 Modeling and fitting ********************** In order to fully understand observations after initial analysis on the image, it is very important to compare them with the existing models to be able to further understand both the models and the data. The tools in this chapter create model galaxies and will provide 2D fittings to be able to understand the detections. * Menu: * MakeProfiles:: Making mock galaxies and stars. * MakeNoise:: Make (add) noise to an image.  File: gnuastro.info, Node: MakeProfiles, Next: MakeNoise, Prev: Modeling and fittings, Up: Modeling and fittings 8.1 MakeProfiles ================ MakeProfiles will create mock astronomical profiles from a catalog, either individually or together in one output image. In data analysis, making a mock image can act like a calibration tool, through which you can test how successfully your detection technique is able to detect a known set of objects. There are commonly two aspects to detecting: the detection of the fainter parts of bright objects (which in the case of galaxies fade into the noise very slowly) or the complete detection of an over-all faint object. Making mock galaxies is the most accurate (and idealistic) way these two aspects of a detection algorithm can be tested. You also need mock profiles in fitting known functional profiles with observations. MakeProfiles was initially built for extra galactic studies, so currently the only astronomical objects it can produce are stars and galaxies. We welcome the simulation of any other astronomical object. The general outline of the steps that MakeProfiles takes are the following: 1. Build the full profile out to its truncation radius in a possibly over-sampled array. 2. Multiply all the elements by a fixed constant so its total magnitude equals the desired total magnitude. 3. If ‘--individual’ is called, save the array for each profile to a FITS file. 4. If ‘--nomerged’ is not called, add the overlapping pixels of all the created profiles to the output image and abort. Using input values, MakeProfiles adds the World Coordinate System (WCS) headers of the FITS standard to all its outputs (except PSF images!). For a simple test on a set of mock galaxies in one image, there is no need for the third step or the WCS information. However in complicated simulations like weak lensing simulations, where each galaxy undergoes various types of individual transformations based on their position, those transformations can be applied to the different individual images with other programs. After all the transformations are applied, using the WCS information in each individual profile image, they can be merged into one output image for convolution and adding noise. * Menu: * Modeling basics:: Astronomical modeling basics. * If convolving afterwards:: Considerations for convolving later. * Flux Brightness and magnitude:: About these measures of energy. * Profile magnitude:: Definition of total profile magnitude. * Invoking astmkprof:: Inputs and Options for MakeProfiles.  File: gnuastro.info, Node: Modeling basics, Next: If convolving afterwards, Prev: MakeProfiles, Up: MakeProfiles 8.1.1 Modeling basics --------------------- In the subsections below, first a review of some very basic information and concepts behind modeling a real astronomical image is given. You can skip this subsection if you are already sufficiently familiar with these concepts. * Menu: * Defining an ellipse:: Defining an ellipse in 2D. * PSF:: Radial profiles for the PSF. * Stars:: Making mock star profiles. * Galaxies:: Radial profiles for galaxies. * Sampling from a function:: Sample a function on a pixelated canvas. * Oversampling:: Oversampling the model.  File: gnuastro.info, Node: Defining an ellipse, Next: PSF, Prev: Modeling basics, Up: Modeling basics 8.1.1.1 Defining an ellipse ........................... The PSF, see *note PSF::, and galaxy radial profiles are generally defined on an ellipse so in this section first defining an ellipse on a pixelated 2D surface is discussed. Labeling the major axis of an ellipse $a$, and its minor axis with $b$, the axis ratio is defined as: $q\equiv b/a$. The major axis of an ellipse can be aligned in any direction, therefore define the angle of the major axis to the horizontal axis of the image is defined to be the position angle of the ellipse and in this book, we show it with $\theta$. Our aim is to put a radial profile of any functional form $f(r)$ over an ellipse. Let’s define the radial distance $r_{el}$ as the distance on the major axis to the center of the ellipse which is located at $x_c$ and $y_c$. We want to find the elliptical distance of a point located at $(i,j)$, in the image coordinate system, from the center of the ellipse. First the coordinate system is rotated by $\theta$ to get the new rotated coordinates of that point $(i_r,j_r)$: $$i_r(i,j)=(i_c-i)\cos(\theta)+(j_c-j)\sin(\theta)$$ $$j_r(i,j)=(j_c-j)\cos(\theta)-(i_c-i)\sin(\theta)$$ The elliptical distance of a point located at $(i,j)$ can now be defined as: $r_{el}^2=\sqrt{i_r^2+j_r^2/q^2} $. To place the radial profiles explained below over an ellipse, $f(r_{el}(i,j))$ is calculated based on the functional radial profile desired. The way MakeProfiles builds the profile is that the nearest pixel in the image to the given profile center is found and the profile value is calculated for it, see *note Sampling from a function::. The next pixel which the profile value is calculated on is the next nearest neighbor of the initial pixel to the profile center (as defined by $r_{el}$). This is done fairly efficiently using a breadth first parsing strategy(1) which is implemented through an ordered linked list. Using this approach, we only go over one layer of pixels on the circumference of the profile to build the profile. Not one more extra pixel has to be checked. Another consequence of this strategy is that extending MakeProfiles to three dimensions becomes very simple: only the neighbors of each pixel have to be changed. Everything else after that (when the pixel index and its radial profile have entered the linked list) is the same, no matter the number of dimensions we are dealing with. ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: PSF, Next: Stars, Prev: Defining an ellipse, Up: Modeling basics 8.1.1.2 Point Spread Function ............................. Assume we have a ‘point’ source, or a source that is far smaller than the maximum resolution (a pixel). When we take an image of it, it will ‘spread’ over an area. To quantify that spread, we can define a ‘function’. This is how the point spread function or the PSF of an image is defined. This ‘spread’ can have various causes, for example in ground based astronomy, due to the atmosphere. In practice we can never surpass the ‘spread’ due to the diffraction of the lens aperture. Various other effects can also be quantified through a PSF. For example, the simple fact that we are sampling in a discrete space, namely the pixels, also produces a very small ‘spread’ in the image. Convolution is the mathematical process by which we can apply a ‘spread’ to an image, or in other words blur the image, see *note Convolution process::. The Brightness of an object should remain unchanged after convolution, see *note Flux Brightness and magnitude::. Therefore, it is important that the sum of all the pixels of the PSF be unity. The PSF image also has to have an odd number of pixels on its sides so one pixel can be defined as the center. In MakeProfiles, the PSF can be set by the two methods explained below. Parametric functions A known mathematical function is used to make the PSF. In this case, only the parameters to define the functions are necessary and MakeProfiles will make a PSF based on the given parameters for each function. In both cases, the center of the profile has to be exactly in the middle of the central pixel of the PSF (which is automatically done by MakeProfiles). When talking about the PSF, usually, the full width at half maximum or FWHM is used as a scale of the width of the PSF. ‘Gaussian’ In the older papers, and to a lesser extent even today, some researchers use the 2D Gaussian function to approximate the PSF of ground based images. In its most general form, a Gaussian function can be written as: $$f(r)=a \exp \left( -(x-\mu)^2 \over 2\sigma^2 \right)+d$$ Since the center of the profile is pre-defined, $\mu$ and $d$ are constrained. $a$ can also be found because the function has to be normalized. So the only important parameter for MakeProfiles is the $\sigma$. In the Gaussian function we have this relation between the FWHM and $\sigma$: $$\rm{FWHM}_g=2\sqrt{2\ln{2}}\sigma \approx 2.35482\sigma$$ ‘Moffat’ The Gaussian profile is much sharper than the images taken from stars on photographic plates or CCDs. Therefore in 1969, Moffat proposed this functional form for the image of stars: $$f(r)=a \left[ 1+\left( r\over \alpha \right)^2 \right]^{-\beta}$$ Again, $a$ is constrained by the normalization, therefore two parameters define the shape of the Moffat function: $\alpha$ and $\beta$. The radial parameter is $\alpha$ which is related to the FWHM by $$\rm{FWHM}_m=2\alpha\sqrt{2^{1/\beta}-1}$$ Comparing with the PSF predicted from atmospheric turbulence theory with a Moffat function, Trujillo et al.(1) claim that $\beta$ should be 4.765. They also show how the Moffat PSF contains the Gaussian PSF as a limiting case when $\beta\to\infty$. An input FITS image An input image file can also be specified to be used as a PSF. If the sum of its pixels are not equal to 1, the pixels will be multiplied by a fraction so the sum does become 1. While the Gaussian is only dependent on the FWHM, the Moffat function is also dependent on $\beta$. Comparing these two functions with a fixed FWHM gives the following results: • Within the FWHM, the functions don’t have significant differences. • For a fixed FWHM, as $\beta$ increases, the Moffat function becomes sharper. • The Gaussian function is much sharper than the Moffat functions, even when $\beta$ is large. ---------- Footnotes ---------- (1) Trujillo, I., J. A. L. Aguerri, J. Cepa, and C. M. Gutierrez (2001). “The effects of seeing on Sérsic profiles - II. The Moffat PSFâ€. In: MNRAS 328, pp. 977—985.  File: gnuastro.info, Node: Stars, Next: Galaxies, Prev: PSF, Up: Modeling basics 8.1.1.3 Stars ............. In MakeProfiles, stars are generally considered to be a point source. This is usually the case for extra galactic studies, were nearby stars are also in the field. Since a star is only a point source, we assume that it only fills one pixel prior to convolution. In fact, exactly for this reason, in astronomical images the light profiles of stars are one of the best methods to understand the shape of the PSF and a very large fraction of scientific research is preformed by assuming the shapes of stars to be the PSF of the image.  File: gnuastro.info, Node: Galaxies, Next: Sampling from a function, Prev: Stars, Up: Modeling basics 8.1.1.4 Galaxies ................ Today, most practitioners agree that the flux of galaxies can be modeled with one or a few generalized de Vaucouleur’s (or Sérsic) profiles. $$I(r) = I_e \exp \left ( -b_n \left[ \left( r \over r_e \right)^{1/n} -1 \right] \right )$$ Gérard de Vaucouleurs (1918-1995) was first to show in 1948 that this function best fits the galaxy light profiles, with the only difference that he held $n$ fixed to a value of 4. 20 years later in 1968, J. L. Sérsic showed that $n$ can have a variety of values and does not necessarily need to be 4. This profile depends on the effective radius ($r_e$) which is defined as the radius which contains half of the profile brightness (see *note Profile magnitude::). $I_e$ is the flux at the effective radius. The Sérsic index $n$ is used to define the concentration of the profile within $r_e$ and $b_n$ is a constant dependent on $n$. MacArthur et al.(1) show that for $n>0.35$, $b_n$ can be accurately approximated using this equation: $$b_n=2n - {1\over 3} + {4\over 405n} + {46\over 25515n^2} + {131\over 1148175n^3}-{2194697\over 30690717750n^4}$$ ---------- Footnotes ---------- (1) MacArthur, L. A., S. Courteau, and J. A. Holtzman (2003). “Structure of Disk-dominated Galaxies. I. Bulge/Disk Parameters, Simulations, and Secular Evolutionâ€. In: ApJ 582, pp. 689—722.  File: gnuastro.info, Node: Sampling from a function, Next: Oversampling, Prev: Galaxies, Up: Modeling basics 8.1.1.5 Sampling from a function ................................ A pixel is the ultimate level of accuracy to gather data, we can’t get any more accurate in one image, this is known as sampling in signal processing. However, the mathematical profiles which describe our models have infinite accuracy. Over a large fraction of the area of astrophysically interesting profiles (for example galaxies or PSFs), the variation of the profile over the area of one pixel is not too significant. In such cases, the elliptical radius ($r_{el}$ of the center of the pixel can be assigned as the final value of the pixel, see *note Defining an ellipse::). As you approach their center, some galaxies become very sharp (their value significantly changes over one pixel’s area). This sharpness increases with smaller effective radius and larger Sérsic values. Thus rendering the central value extremely inaccurate. The first method that comes to mind for solving this problem is integration. The functional form of the profile can be integrated over the pixel area in a 2D integration process. However, unfortunately numerical integration techniques also have their limitations and when such sharp profiles are needed they can become extremely inaccurate. The most accurate method of sampling a continuous profile on a discrete space is by choosing a large number of random points within the boundaries of the pixel and taking their average value (or Monte Carlo integration). This is also, generally speaking, what happens in practice with the photons on the pixel. The number of random points can be set with ‘--numrandom’. Unfortunately, repeating this Monte Carlo process would be extremely time and CPU consuming if it is to be applied to every pixel. In order to not loose too much accuracy, in MakeProfiles, the profile is built using both methods explained above. The building of the profile begins from its central pixel and continues outwards. Monte Carlo integration is first applied (which yields $F_r$), then the central pixel value ($F_c$) on the same pixel. If the fractional difference ($|F_r-F_c|/F_r$) is lower than a given tolerance level we will stop using Monte Carlo integration and only use the central pixel value. The ordering of the pixels in this inside-out construction is based on $r=\sqrt{(i_c-i)^2+(j_c-j)^2}$, not $r_{el}$, see *note Defining an ellipse::. When the axis ratios are large (near one) this is fine. But when they are small and the object is highly elliptical, it might seem more reasonable to follow $r_{el}$ not $r$. The problem is that the gradient is stronger in pixels with smaller $r$ (and larger $r_{el}$) than those with smaller $r_{el}$. In other words, the gradient is strongest along the minor axis. So if the next pixel is chosen based on $r_{el}$, the tolerance level will be reached sooner and lots of pixels with large fractional differences will be missed. Monte Carlo integration uses a random number of points. Thus, every time you run it, by default, you will get a different distribution of points to sample within the pixel. In the case of large profiles, this will result in a slight difference of the pixels which use Monte Carlo integration each time MakeProfiles is run. To have a deterministic result, you have to fix the random number generator properties which is used to build the random distribution. This can be done by setting the ‘GSL_RNG_TYPE’ and ‘GSL_RNG_SEED’ environment variables and calling MakeProfiles with the ‘--envseed’ option. To learn more about the process of generating random numbers, see *note Generating random numbers::. The seed values are fixed for every profile: with ‘--envseed’, all the profiles have the same seed and without it, each will get a different seed using the system clock (which is accurate to within one microsecond). The same seed will be used to generate a random number for all the sub-pixel positions of all the profiles. So in the former, the sub-pixel points checked for all the pixels undergoing Monte carlo integration in all profiles will be identical. In other words, the sub-pixel points in the first (closest to the center) pixel of all the profiles will be identical with each other. All the second pixels studied for all the profiles will also receive an identical (different from the first pixel) set of sub-pixel points and so on. As long as the number of random points used is large enough or the profiles are not identical, this should not cause any systematic bias.  File: gnuastro.info, Node: Oversampling, Prev: Sampling from a function, Up: Modeling basics 8.1.1.6 Oversampling .................... The steps explained in *note Sampling from a function:: do give an accurate representation of a profile prior to convolution. However, in an actual observation, the image is first convolved with or blurred by the atmospheric and instrument PSF in a continuous space and then it is sampled on the discrete pixels of the camera. In order to more accurately simulate this process, the unconvolved image and the PSF are created on a finer pixel grid. In other words, the output image is a certain odd-integer multiple of the desired size, we can call this ‘oversampling’. The user can specify this multiple as a command-line option. The reason this has to be an odd number is that the PSF has to be centered on the center of its image. An image with an even number of pixels on each side does not have a central pixel. The image can then be convolved with the PSF (which should also be oversampled on the same scale). Finally, image can be sub-sampled to get to the initial desired pixel size of the output image. After this, mock noise can be added as explained in the next section. This is because unlike the PSF, the noise occurs in each output pixel, not on a continuous space like all the prior steps.  File: gnuastro.info, Node: If convolving afterwards, Next: Flux Brightness and magnitude, Prev: Modeling basics, Up: MakeProfiles 8.1.2 If convolving afterwards ------------------------------ In case you want to convolve the image later with a given point spread function, make sure to use a larger image size. After convolution, the profiles become larger and a profile that is normally completely outside of the image might fall within it. On one axis, if you want your final (convolved) image to be $m$ pixels and your PSF is $2n+1$ pixels wide, then when calling MakeProfiles, set the axis size to $m+2n$, not $m$. You also have to shift all the pixel positions of the profile centers on the that axis by $n$ pixels to the positive. After convolution, you can crop the outer $n$ pixels with the section crop box specification of ImageCrop: ‘--section=n:*-n,n:*-n’ assuming your PSF is a square, see *note Crop section syntax::. This will also remove all discrete Fourier transform artifacts (blurred sides) from the final image. To facilitate this shift, MakeProfiles has the options ‘--xshift’, ‘--yshift’ and ‘--prepforconv’, see *note Invoking astmkprof::.  File: gnuastro.info, Node: Flux Brightness and magnitude, Next: Profile magnitude, Prev: If convolving afterwards, Up: MakeProfiles 8.1.3 Flux Brightness and magnitude ----------------------------------- Astronomical data pixels are usually in units of counts(1) or electrons or either one divided by seconds. To convert from the counts to electrons, you will need to know the instrument gain. In any case, they can be directly converted to energy or energy/time using the basic hardware (telescope, camera and filter) information. We will continue the discussion assuming the pixels are in units of energy/time. The _brightness_ of an object is defined as its total detected energy per time. This is simply the sum of the pixels that are associated with that detection by our detection tool for example *note NoiseChisel::(2). The _flux_ of an object is in units of energy/time/area and for a detected object, it is defined as its brightness divided by the area used to collect the light from the source or the telescope aperture (for example in $cm^2$)(3). Knowing the flux ($f$) and distance to the object ($r$), we can calculate its _luminosity_: $L=4{\pi}r^2f$. Therefore, flux and luminosity are intrinsic properties of the object, while brightness depends on our detecting tools (hardware and software). Here we will not be discussing luminosity, but brightness. However, since luminosity is the astrophysically interesting quantity, we also defined it here to avoid possible confusion between these two terms because they both have the same units. Images of astronomical objects span over a very large range of brightness. With the Sun (as the brightest object) being roughly $2.5^{60}=10^{24}$ times brighter than the faintest galaxies we can currently detect. Therefore discussing brightness will be very hard, and astronomers have chosen to use a logarithmic scale to talk about the brightness of astronomical objects. But the logarithm can only be usable with a unit-less and always positive value. Fortunately brightness is always positive and to remove the units we divide the brightness of the object ($B$) by a reference brightness ($B_r$). We then define the resulting logarithmic scale as $magnitude$ through the following relation(4) $$m-m_r=-2.5\log_{10} \left( B \over B_r \right)$$ $m$ is defined as the magnitude of the object and $m_r$ is the pre-defined magnitude of the reference brightness. One particularly easy condition is when $B_r=1$. This will allow us to summarize all the hardware specific parameters discussed above into one number as the reference magnitude which is commonly known as the Zero-point(5) magnitude. ---------- Footnotes ---------- (1) Counts are also known as analog to digital units (ADU). (2) If further processing is done, for example the Kron or Petrosian radii are calculated, then the detected area is not sufficient and the total area that was within the respective radius must be used. (3) For a full object that spans over several pixels, the telescope area should be used to find the flux. However, sometimes, only the brightness per pixel is desired. In such cases this book also _loosely_ uses the term flux. This is only approximately accurate however, since while all the pixels have a fixed area, the pixel size can vary with camera on the telescope. (4) The $-2.5$ factor in the definition of magnitudes is a legacy of the our ancient colleagues and in particular Hipparchus of Nicaea (190-120 BC). (5) When $B=Br=1$, the right side of the magnitude definition will be zero. Hence the name, “zero-pointâ€.  File: gnuastro.info, Node: Profile magnitude, Next: Invoking astmkprof, Prev: Flux Brightness and magnitude, Up: MakeProfiles 8.1.4 Profile magnitude ----------------------- To find the profile brightness or its magnitude, (see *note Flux Brightness and magnitude::), it is customary to use the 2D integration of the flux to infinity. However, in MakeProfiles we do not follow this idealistic approach and apply a more realistic method to find the total brightness or magnitude: the sum of all the pixels belonging to a profile within its predefined truncation radius. Note that if the truncation radius is not large enough, this can be significantly different from the total integrated light to infinity. An integration to infinity is not a realistic condition because no galaxy extends indefinitely (important for high Sérsic index profiles), pixelation can also cause a significant difference between the actual total pixel sum value of the profile and that of integration to infinity, especially in small and high Sérsic index profiles. To be safe, you can specify a large enough truncation radius for such compact high Sérsic index profiles. If oversampling is used then the brightness is calculated using the over-sampled image, see *note Oversampling:: which is much more accurate. The profile is first built in an array completely bounding it with a normalization constant of unity (see *note Galaxies::). Taking $B$ to be the desired brightness and $S$ to be the sum of the pixels in the created profile, every pixel is then multiplied by $B/S$ so the sum is exactly $B$. If the ‘--individual’ option is called, this same array is written to a FITS file. If not, only the overlapping pixels of this array and the output image are kept and added to the output array.  File: gnuastro.info, Node: Invoking astmkprof, Prev: Profile magnitude, Up: MakeProfiles 8.1.5 Invoking MakeProfiles --------------------------- MakeProfiles will make any number of profiles specified in a catalog either individually or in one image. The executable name is ‘astmkprof’ with the following general template $ astmkprof [OPTION ...] [BackgroundImage] Catalog One line examples: $ astmkprof background.fits catalog.txt $ astmkprof --xcol=0 --ycol=1 catalog.txt $ astmkprof --individual --oversample 3 -x500 -y500 catalog.txt If mock images are to be made, the catalog (which stores the parameters for each mock profile) is the mandatory argument. The input catalog has to be a text file formatted in a table with columns separated by space, tab or comma (<,>) characters. See *note Common program behavior:: for a complete explanation of some common behaviour and options in all Gnuastro programs including MakeProfiles. If a data image file (see *note Arguments::) is given, the pixels of that image are used as the background value for every pixel. The flux value of each profile pixel will be added to the pixel in that background value. In this case the values to all options relating to the output size and WCS will be ignored if specified (for example ‘--naxis1’, ‘--naxis2’ and ‘--prepforconv’) on the command-line or in the configuration files. Note that ‘--oversample’ will remain active even if a background image is specified. * Menu: * MakeProfiles catalog:: Required catalog properties. * MakeProfiles options:: Full list of MakeProfiles options. * MakeProfiles output:: The generated outputs.  File: gnuastro.info, Node: MakeProfiles catalog, Next: MakeProfiles options, Prev: Invoking astmkprof, Up: Invoking astmkprof 8.1.5.1 MakeProfiles catalog ............................ The catalog is a text file table. Its columns can be ordered in any desired manner, you can specify which columns belong to which parameters using the set of options ending with ‘col’, for example ‘--xcol’ or ‘--rcol’, see *note MakeProfiles options::. The value for the profile center in the catalog (in the ‘--xcol’ and ‘--ycol’ columns) can be a floating point number so the profile center can be on any sub-pixel position. Note that pixel positions in the FITS standard start from 1 and an integer is the pixel center. So a 2D image actually starts from the position (0.5, 0.5). In MakeProfiles profile centers do not have to be in the image. Even if only one pixel of the profile within the truncation radius is within the output image, that pixel is included in the image. Profiles that are completely out of the image will not be created. You can use the output log file to see which profiles were within the image. If PSF profiles (Moffat or Gaussian) are in the catalog and the profiles are to be built in one image (when ‘--individual’ is not used), it is assumed they are the PSF(s) you want to convolve your created image with. So by default, they will not be built in the output image but as separate files. The sum of pixels of these separate files will also be set to unity (1) so you are ready to convolve, see *note Convolution process::. As a summary, their position and magnitude will be ignored. This behaviour can be disabled with the ‘--psfinimg’ option. If you want to create all the profiles separately (with ‘--individual’) and you want the sum of the PSF profile pixels to be unity, you have to set their magnitudes in the catalog to the zero-point magnitude and be sure that the central positions of the profiles don’t have any fractional part (the PSF center has to be in the center of the pixel).  File: gnuastro.info, Node: MakeProfiles options, Next: MakeProfiles output, Prev: MakeProfiles catalog, Up: Invoking astmkprof 8.1.5.2 MakeProfiles options ............................ The common options that are shared by Gnuastro programs, are fully explained in *note Common options:: and are not repeated here. Since there are no image inputs, the‘--hdu’ option is ignored. The options can be classified into the following categories: Output, Profiles, Catalog and WCS. Below each one is reviewed. Output: ‘-x’ ‘--naxis1’ (‘=INT’) The number of pixels in the output image along the first FITS axis (horizontal when viewed in SAO ds9). This is before over-sampling. For example if you call MakeProfiles with ‘--naxis1=100 --oversample=5’ (assuming no shift due for later convolution), then the final image size along the first axis will be 500. If a background image is specified, any possible value to this option is ignored. ‘-y’ ‘--naxis2’ (‘=INT’) The number of pixels in the output image along the second FITS axis (vertical when viewed in SAO ds9), see the explanation for ‘--naxis1’. ‘-T’ ‘--type’ (‘=STR’) Type of the output image pixels (specified by ‘BITPIX’ in the FITS standard). It can have any one of the following values: ‘byte’, ‘short’, ‘long’, ‘longlong’, ‘float’, ‘double’. Internally, the images are made in the float type, but upon writing of the single output (not individual profiles), the image will be converted to the type specified by this option. When a background image is given without the ‘--inputascanvas’ option, it is assumed that you want the output in the same format as the background, therefore the value to this option is ignored. ‘-C’ ‘--inputascanvas’ When an image is given as an argument, use the input image as the canvas to make all the mock profiles. In practice, this option only changes the non-blank pixels (see *note Blank pixels::) of the input image (in memory after reading, not the actual input file) to zero before making the profiles. The profiles are then built on those cleared pixels. With this option (like when building on a background image) the values to ‘--naxis1’, ‘--naxis2’, ‘--crpix1’, ‘--crpix2’, ‘--crval1’, ‘--crval2’, and ‘--resolution’ are ignored. However, if ‘--type’ is given, its value will take precedence over the background image type. This option can be very useful when the mock image is to be made over a real sky region and compared to a real image (that might have blank pixels. One example can be when you want to make circular or elliptical labeled regions to feed into MakeCatalog along with NoiseChisel’s outputs for aperture photometry. See the discussion and examples under the ‘‘--mforflatpix’’ for more. ‘-s’ ‘--oversample’ (‘=INT’) The scale to over-sample the profiles and final image. If not an odd number, will be added by one, see *note Oversampling::. Note that this ‘--oversample’ will remain active even if an input image is specified. If your input catalog is based on the background image, be sure to set ‘--oversample=1’. ‘--psfinimg’ Build the possibly existing PSF profiles (Moffat or Gaussian) in the catalog into the final image. By default they are built separately so you can convolve your images with them, thus their magnitude and positions are ignored. With this option, they will be built in the final image like every other galaxy profile. To have a final PSF in your image, make a point profile where you want the PSF and after convolution it will be the PSF. ‘-i’ ‘--individual’ If this option is called, each profile is created in a separate FITS file within the same directory as the output and the row number of the profile (starting from zero) in the name. The file for each row’s profile will be in the same directory as the final combined image of all the profiles and will have the final image’s name as a suffix. So for example if the final combined image is named ‘./out/fromcatalog.fits’, then the first profile that will be created with this option will be named ‘./out/0_fromcatalog.fits’. Since each image only has one full profile out to the truncation radius the profile is centered and so, only the sub-pixel position of the profile center is important for the outputs of this option. The output will have an odd number of pixels. If there is no oversampling, the central pixel will contain the profile center. If the value to ‘--oversample’ is larger than unity, then the profile center is on any of the central ‘--oversample’’d pixels depending on the fractional value of the profile center. If the fractional value is larger than half, it is on the bottom half of the central region. This is due to the FITS definition of a real number position: The center of a pixel has fractional value $0.00$ so each pixel contains these fractions: .5 – .75 – .00 (pixel center) – .25 – .5. ‘-m’ ‘--nomerged’ Don’t make a merged image. By default after making the profiles, they are added to a final image with sides of ‘--naxis1’ and ‘--naxis2’ if they overlap with it. Profiles: ‘-r’ ‘--numrandom’ The number of random points used in the central regions of the profile, see *note Sampling from a function::. ‘-e’ ‘--envseed’ Use the value to the ‘GSL_RNG_SEED’ environment variable to generate the random Monte Carlo sampling distribution, see *note Sampling from a function:: and *note Generating random numbers::. ‘-t’ ‘--tolerance’ (‘=FLT’) The tolerance to switch from Monte Carlo integration to the central pixel value, see *note Sampling from a function::. ‘-p’ ‘--tunitinp’ The truncation column of the catalog is in units of pixels. By default, the truncation column is considered to be in units of the radial parameters of the profile (‘--rcol’). Read it as ‘t-unit-in-p’ for ‘truncation unit in pixels’. ‘-X’ ‘--xshift’ (‘=INT’) Shift all the profiles and enlarge the image along the first FITS axis, see $n$ in *note If convolving afterwards::. This is useful when you want to convolve the image afterwards. If you are using an external PSF, be sure to oversample it to the same scale used for creating the mock images. If a background image is specified, any possible value to this option is ignored. ‘-Y’ ‘--yshift’ (‘=INT’) Similar to ‘--xshift’ for the second FITS axis. ‘-c’ ‘--prepforconv’ Shift all the profiles and enlarge the image based on half the width of the first Moffat or Gaussian profile in the catalog, considering any possible oversampling see *note If convolving afterwards::. ‘--prepforconv’ is only checked and possibly activated if ‘--xshift’ and ‘--yshift’ are both zero (after reading the command-line and configuration files). If a background image is specified, any possible value to this option is ignored. ‘--magatpeak’ The magnitude column in the catalog (see *note MakeProfiles catalog::) will be used to find the brightness only for the peak profile pixel, not the full profile. Note that this is the flux of the profile’s peak pixel in the final output of MakeProfiles. So beware of the oversampling, see *note Oversampling::. This option can be useful if you want to check a mock profile’s total magnitude at various truncation radii. Without this option, no matter what the truncation radius is, the total magnitude will be the same as that given in the catalog. But with this option, the total magnitude will become brighter as you increase the truncation radius. In sharper profiles, sometimes the accuracy of measuring the peak profile flux is more than the overall object brightness. In such cases, with this option, the final profile will be built such that its peak has the given magnitude, not the total profile. *CAUTION:* If you want to use this option for comparing with observations, please note that MakeProfiles does not do convolution. Unless you have de-convolved your data, your images are convolved with the instrument and atmospheric PSF, see *note PSF::. Particularly in sharper profiles, the flux in the peak pixel is strongly decreased after convolution. Also note that in such cases, besides de-convolution, you will have to set ‘--oversample=1’ otherwise after resampling your profile with ImageWarp (see *note ImageWarp::), the peak flux will be different. ‘-R’ ‘--replace’ Do not add the pixels of each profile over the background (possibly crowded by other profiles), replace them. By default, when two profiles overlap, the final pixel value is the sum of all the profiles that overlap on that pixel. When this option is given, the pixels are not added but replaced by the newer profile’s pixel and any value under it is lost. When order matters, make sure to use this function with ‘‘--numthreads=1’’. When multiple threads are used, the separate profiles are built asynchronously and not in order. Since order does not matter in an addition, this causes no problems by default but has to be considered when this option is given. Using multiple threads is no problem if the profiles are to be used as a mask with a blank or fixed value (see ‘‘--mforflatpix’’) since all their pixel values are the same. Note that only non-zero pixels are replaced. With radial profiles (for example Sérsic or Moffat) only values above zero will be part of the profile. However, when using flat profiles with the ‘‘--mforflatpix’’ option, you should be careful not to give a ‘0.0’ value as the flat profile’s pixel value. ‘-w’ ‘--circumwidth’ (‘=FLT’) The width of the circumference if the profile is to be an elliptical circumference or annulus. See the explanations for this type of profile in ‘--fcol’. ‘-z’ ‘--zeropoint’ (‘=FLT’) The zero-point magnitude of the image. Catalog: The value to all of these options is considered to be a column number, where counting starts from zero. ‘--fcol’ (‘=INT’) The functional form of the profile with one of the values below. Note that this value will be converted to an integer before analysis using the internal type conversion of C. So for example 2.80 will be converted to 2. • 0: Sérsic. • 1: Moffat. • 2: Gaussian. • 3: Point source (a star). • 4: Flat profile: all pixels have same value. • 5: Circumference: same value for all pixels between the truncation radius ($r_t$) and $r_t-w$ where $w$ is the value to the ‘--circumwidth’. Currently this is only intended to be used for making an elliptical annulus (with a width of 1 or 2 pixels). ‘--xcol’ (‘=INT’) The center of the profiles along the first FITS axis (horizontal when viewed in SAO ds9). See the explanations for ‘--racol’ for precedence when both image and WCS coordinate columns are given. ‘--ycol’ (‘=INT’) The center of the profiles along the second FITS axis (vertical when viewed in SAO ds9). Similar to ‘--xcol’. ‘--racol’ (‘=INT’) The profile center’s right ascension. Along with ‘--deccol’, these WCS coordinate columns are not mandatory. If they are not given, the ‘--xcol’ and ‘--ycol’ options will be used to specify the profile’s central position and vice-versa. However, if image coordinate columns (‘--xcol’ and ‘--ycol’) and WCS coordinate columns (‘--racol’ and ‘--deccol’) are given, the WCS coordinate columns take precedence and image coordinate columns will be ignored. ‘--deccol’ (‘=INT’) The profile center’s declination. Similar to ‘--racol’. ‘--rcol’ (‘=INT’) The radius parameter of the profiles. Effective radius ($r_e$) if Sérsic, FWHM if Moffat or Gaussian. ‘--ncol’ (‘=INT’) The Sérsic index ($n$) or Moffat $\beta$. ‘--pcol’ (‘=INT’) The position angle (in degrees) of the profiles relative to the first FITS axis (horizontal when viewed in SAO ds9). ‘--qcol’ (‘=INT’) The axis ratio of the profiles (minor axis divided by the major axis). ‘--mcol’ (‘=INT’) The total pixelated magnitude of the profile within the truncation radius, see *note Profile magnitude::. ‘--tcol’ (‘=INT’) The truncation radius of this profile. By default it is in units of the radial parameter of the profile (the value in the ‘--rcol’ of the catalog). If ‘--tunitinp’ is given, this value is interpreted in units of pixels (prior to oversampling) irrespective of the profile. ‘-F’ ‘--mforflatpix’ When making fixed value profiles (flat and circumference, see ‘‘--fcol’’), don’t use the value in the column specified by ‘‘--mcol’’ as the magnitude. Instead use it as the exact value that all the pixels of these profiles should have. This option is irrelevant for other types of profiles. This option is very useful for creating masks, or labeled regions in an image. Any integer, or floating point value can used in this column with this option, including ‘NaN’ (or ‘‘nan’’, or ‘‘NAN’’, case is irrelevant), and infinities (‘inf’, ‘-inf’, or ‘+inf’). For example, with this option if you set the value in the magnitude column (‘--mcol’) to ‘NaN’, you can create an elliptical or circular mask over an image (which can be given as the argument), see *note Blank pixels::. Another useful application of this option is to create labeled elliptical or circular apertures in an image. To do this, set the value in the magnitude column to the label you want for this profile. This labeled image can then be used in combination with NoiseChisel’s output (see *note NoiseChisel output::) to do aperture photometry with MakeCatalog (see *note MakeCatalog::). Alternatively, if you want to mark regions of the image (for example with an elliptical circumference) and you don’t want to use NaN values (as explained above) for some technical reason, you can get the minimum or maximum value in the image (1) using Arithmetic (see *note Arithmetic::), then use that value in the magnitude column along with this option for all the profiles. Please note that when using MakeProfiles on an already existing image, you have to set ‘‘--oversample=1’’. Otherwise all the profiles will be scaled up based on the oversampling scale in your configuration files (see *note Configuration files::) unless you have accounted for oversampling in your catalog. WCS: ‘--crpix1’ (‘=FLT’) The pixel coordinates of the WCS reference point on the first (horizontal) FITS axis (counting from 1). ‘--crpix2’ (‘=FLT’) The pixel coordinates of the WCS reference point on the second (vertical) FITS axis (counting from 1). ‘--crval1’ (‘=FLT’) The Right Ascension (RA) of the reference point. ‘--crval2’ (‘=FLT’) The Declination of the reference point. ‘--resolution’ (‘=FLT’) The resolution of the non-oversampled image in units of arcseconds/pixel. ---------- Footnotes ---------- (1) The minimum will give a better result, because the maximum can be too high compared to most pixels in the image, making it harder to display.  File: gnuastro.info, Node: MakeProfiles output, Prev: MakeProfiles options, Up: Invoking astmkprof 8.1.5.3 MakeProfiles output ........................... Besides the final merged image of all the profiles or individual profiles that can be built based on the input options, MakeProfiles will also create a log file in the current directory (where you run MockProfiles). The values for each column are explained in the first few commented (starting with ‘#’ character). The log file includes the following information: • The total magnitude of the profile in the image. This will be different from your input magnitude if the profile was not completely in the image. • The number of pixels (in the oversampled image) which used Monte Carlo integration and not the central pixel value. • The fraction of flux in the Monte Carlo integrated pixels. • If an individual image was created or not.  File: gnuastro.info, Node: MakeNoise, Prev: MakeProfiles, Up: Modeling and fittings 8.2 MakeNoise ============= Real data are always buried in noise, therefore to finalize a simulation of real data (for example to test our observational algorithms) it is essential to add noise to the mock profiles created with MakeProfiles, see *note MakeProfiles::. Below, the general principles and concepts to help understand how noise is quantified is discussed. MakeNoise options and argument are then discussed in *note Invoking astmknoise::. * Menu: * Noise basics:: Noise concepts and definitions. * Invoking astmknoise:: Options and arguments to MakeNoise. gnuastro-0.2.33-8a3b/doc/gnuastro.info-10000644000175000017500000113222313004464700014541 00000000000000This is gnuastro.info, produced by makeinfo version 6.3 from gnuastro.texi. This book documents version 0.2.33-8a3b of the GNU Astronomy Utilities (Gnuastro). Gnuastro provides various programs and libraries for astronomical data manipulation and analysis. Copyright © 2015-2016 Free Software Foundation, Inc. Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled “GNU Free Documentation Licenseâ€. INFO-DIR-SECTION Astronomy START-INFO-DIR-ENTRY * Gnuastro: (gnuastro). GNU Astronomy Utilities. * help-gnuastro: (gnuastro)help-gnuastro mailing list. Getting help. * bug-gnuastro: (gnuastro)Report a bug. How to report bugs * ConvertType: (gnuastro)ConvertType. Convert different file types. * astconvertt: (gnuastro)Invoking astconvertt. Options to ConvertType. * Convolve: (gnuastro)Convolve. Convolve an input file with kernel. * astconvolve: (gnuastro)Invoking astconvolve. Options to Convolve. * CosmicCalculator: (gnuastro)CosmicCalculator. For cosmological params. * astcosmiccal: (gnuastro)Invoking astcosmiccal. Options to CosmicCalculator. * Header: (gnuastro)Header. Print and manipulate data header info. * astheader: (gnuastro)Invoking astheader. Options to Header. * ImageCrop: (gnuastro)ImageCrop. Crop region(s) from image(s). * astimgcrop: (gnuastro)Invoking astimgcrop. Options to ImageCrop. * Arithmetic: (gnuastro)Arithmetic. Arithmetic operations on pixels. * astarithmetic: (gnuastro)Invoking astarithmetic. Options to Arithmetic. * ImageStatistics: (gnuastro)ImageStatistics. Get image Statistics. * astimgstat: (gnuastro)Invoking astimgstat. Options to ImageStatistics. * ImageWarp: (gnuastro)ImageWarp. Warp an image to a new grid. * astimgwarp: (gnuastro)Invoking astimgwarp. Options to ImageWarp. * MakeCatalog: (gnuastro)MakeCatalog. Make a catalog from labeled image. * astmkcatalog: (gnuastro)Invoking astmkcatalog. Options to MakeCatalog. * MakeNoise: (gnuastro)MakeNoise. Make (add) noise to an image. * astmknoise: (gnuastro)Invoking astmkprof. Options to MakeNoise. * MakeProfiles: (gnuastro)MakeProfiles. Make mock profiles. * astmkprof: (gnuastro)Invoking astmkprof. Options to MakeProfiles. * NoiseChisel: (gnuastro)NoiseChisel. Detect signal in noise. * astnoisechisel: (gnuastro)Invoking astnoisechisel. Options to NoiseChisel. * SubtractSky: (gnuastro)SubtractSky. Find and subtract the sky value. * astsubtractsky: (gnuastro)Invoking astsubtractsky. Options to SubtractSky. * Table: (gnuastro)Table. Read and write FITS binary or ASCII tables. * asttable: (gnuastro)Invoking asttable. Options to Table. END-INFO-DIR-ENTRY  File: gnuastro.info, Node: Top, Next: Introduction, Prev: (dir), Up: (dir) GNU Astronomy Utilities *********************** This book documents version 0.2.33-8a3b of the GNU Astronomy Utilities (Gnuastro). Gnuastro provides various programs and libraries for astronomical data manipulation and analysis. Copyright © 2015-2016 Free Software Foundation, Inc. Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled “GNU Free Documentation Licenseâ€. * Menu: * Introduction:: General introduction. * Tutorials:: Tutorials or Cookbooks. * Installation:: Requirements and installation. * Common program behavior:: Common behavior in all programs. * Extensions and Tables:: Tools to operate on extensions and tables. * Image manipulation:: Tools for basic image manipulation. * Image analysis:: Analyze images. * Modeling and fittings:: Make and fit models. * High-level calculations:: Physical calculations. * Libraries:: Use Gnuastro in your own code. * Developing:: The development environment. * Gnuastro programs list:: List and short summary of Gnuastro. * Other useful software:: Installing other useful software. * GNU Free Documentation License:: Full FDL text. * Index:: Index of terms — The Detailed Node Listing — Introduction * Quick start:: A quick start to installation. * Science and its tools:: Some philosophy and history. * Your rights:: User rights. * Naming convention:: About names of programs in Gnuastro. * Version numbering:: Understanding version numbers. * New to GNU/Linux?:: Suggested GNU/Linux distribution. * Report a bug:: Search and report the bug you found. * Suggest new feature:: How to suggest a new feature. * Announcements:: How to stay up to date with Gnuastro. * Conventions:: Conventions used in this book. * Acknowledgments:: People who helped in the production. Version numbering * GNU Astronomy Utilities 1.0:: Plans for version 1.0 release New to GNU/Linux? * Command-line interface:: Introduction to the command-line Tutorials * Hubble visually checks and classifies his catalog:: Check a catalog. * Sufi simulates a detection:: Simulating a detection. Installation * Dependencies:: Necessary packages for Gnuastro. * Downloading the source:: Ways to download the source code. * Build and install:: Configure, build and install Gnuastro. Dependencies * Mandatory dependencies:: Gnuastro will not install without these. * Optional dependencies:: Adding more functionality. * Bootstrapping dependencies:: If you have the version controlled source. Mandatory dependencies * GNU Scientific Library:: Installing GSL. * CFITSIO:: C interface to the FITS standard. * WCSLIB:: C interface to the WCS standard of FITS. Downloading the source * Release tarball:: Download a stable official release. * Version controlled source:: Get and use the version controlled source. Version controlled source * Bootstrapping:: Adding all the automaticly generated files. * Synchronizing:: Keep your local clone up to date. Build and install * Configuring:: Configure Gnuastro * Tests:: Run tests to see if it is working. * A4 print book:: Customize the print book. * Known issues:: Issues you might encounter. Configuring * Gnuastro configure options:: Configure options particular to Gnuastro. * Installation directory:: Specify the directory to install. * Executable names:: Changing executable names. * Configure and build in RAM:: For minimal use of HDD or SSD, and clean source. Common program behavior * Command-line:: How to use the command-line. * Configuration files:: Values for unspecified variables. * Threads in Gnuastro:: How threads are managed in Gnuastro. * Final parameter values:: The final set of used parameters. * Automatic output:: About automatic output names. * Getting help:: Getting more information on the go. * Output headers:: Common headers to all FITS outputs. Command-line * Arguments and options:: Basics of options and arguments. * Arguments:: Treatment of arguments. * Options:: How to use GNU style options. * Common options:: Common options to all Gnuastro programs. Common options * Input output:: Common input/output options. * Operating modes:: Common operating mode options. Configuration files * Configuration file format:: ASCII format of configuration file. * Configuration file precedence:: Precedence of configuration files. * Current directory and User wide:: Local and user configuration files. * System wide:: System wide configuration files. Threads in Gnuastro * A note on threads:: Caution and suggestion on using threads. * How to run simultaneous operations:: How to run things simultaneously. Getting help * --usage:: View option names and value formats. * --help:: List all options with description. * Man pages:: Man pages generated from –help. * Info:: View complete book in terminal. * help-gnuastro mailing list:: Contacting experienced users. Extensions and Tables * Header:: Print and manipulate data file header. * ConvertType:: Convert data to various formats. * Table:: Read and Write FITS tables to plain text. Header * Invoking astheader:: Arguments and options to Header. ConvertType * Recognized file types:: Recognized file types * Color:: Some explanations on color. * Invoking astconvertt:: Options and arguments to ConvertType. Table * Invoking asttable:: Options and arguments to Table. Image manipulation * ImageCrop:: Crop region(s) from FITS image(s). * Arithmetic:: Arithmetic on input data. * Convolve:: Convolve an image with a kernel. * ImageWarp:: Warp/Transform an image to a different grid. * SubtractSky:: Find the sky and subtract it from image. ImageCrop * ImageCrop modes:: Basic ImageCrop modes. * Crop section syntax:: How to define a section to crop. * Blank pixels:: Pixels with no value. * Invoking astimgcrop:: Calling ImageCrop on the command-line Invoking ImageCrop * astimgcrop options:: A list of all the options with explanation. * astimgcrop output:: The outputs of ImageCrop. Arithmetic * Reverse polish notation:: The current notation style for Arithmetic * Arithmetic operators:: List of operators known to Arithmetic * Invoking astarithmetic:: How to run Arithmetic: options and output Convolve * Spatial domain convolution:: Only using the input image values. * Frequency domain and Fourier operations:: Using frequencies in input. * Spatial vs. Frequency domain:: When to use which? * Convolution kernel:: How to specify the convolution kernel. * Invoking astconvolve:: Options and argument to Convolve. Spatial domain convolution * Convolution process:: More basic explanations. * Edges in the spatial domain:: Dealing with the edges of an image. Frequency domain and Fourier operations * Fourier series historical background:: Historical background. * Circles and the complex plane:: Interpreting complex numbers. * Fourier series:: Fourier Series definition. * Fourier transform:: Fourier Transform definition. * Dirac delta and comb:: Dirac delta and Dirac comb. * Convolution theorem:: Derivation of Convolution theorem. * Sampling theorem:: Sampling theorem (Nyquist frequency). * Discrete Fourier transform:: Derivation and explanation of DFT. * Fourier operations in two dimensions:: Extend to 2D images. * Edges in the frequency domain:: Interpretation of edge effects. ImageWarp * Warping basics:: Basics of coordinate transformation. * Merging multiple warpings:: How to merge multiple matrices. * Resampling:: Warping an image is re-sampling it. * Invoking astimgwarp:: Arguments and options for ImageWarp. SubtractSky * Sky value:: Definition of the sky value. * Tiling an image:: Defining a mesh grid on the image. * Mask image:: How to mask pixels for no analysis. * Invoking astsubtractsky:: Options and arguments to SubtractSky. Sky value * Finding the sky value:: How SubtractSky finds the sky value. * Sky value misconceptions:: Sky value misconceptions and wrong approaches. Tiling an image * Quantifying signal in a mesh:: Good meshs for gradients. * Grid interpolation and smoothing:: Filling the blank grid elements. * Checking grid values:: Check the values on the grid. * Mesh grid options:: Common options related to the mesh grid. Image analysis * ImageStatistics:: Calculate main image statistics. * NoiseChisel:: Detect objects in an image. * MakeCatalog:: Catalog from input and labeled images. ImageStatistics * Histogram and Cumulative Frequency Plot:: Basic definitions. * Sigma clipping:: Definition of $\sigma$-clipping * Mirror distribution:: Used for finding the mode. * Invoking astimgstat:: Arguments and options to ImageStatistics. NoiseChisel * Invoking astnoisechisel:: Options and arguments for NoiseChisel. Invoking NoiseChisel * NoiseChisel options:: The options specific to NoiseChisel. * NoiseChisel output:: NoiseChisel’s output. Why no catalog? MakeCatalog * Quantifying data limits:: For comparing different catalogs. * Measuring elliptical parameters:: Estimating elliptical parameters. * Invoking astmkcatalog:: Options and arguments to MakeCatalog. * Adding new columns to MakeCatalog:: How to add new columns. Modeling and fitting * MakeProfiles:: Making mock galaxies and stars. * MakeNoise:: Make (add) noise to an image. MakeProfiles * Modeling basics:: Astronomical modeling basics. * If convolving afterwards:: Considerations for convolving later. * Flux Brightness and magnitude:: About these measures of energy. * Profile magnitude:: Definition of total profile magnitude. * Invoking astmkprof:: Inputs and Options for MakeProfiles. Modeling basics * Defining an ellipse:: Defining an ellipse in 2D. * PSF:: Radial profiles for the PSF. * Stars:: Making mock star profiles. * Galaxies:: Radial profiles for galaxies. * Sampling from a function:: Sample a function on a pixelated canvas. * Oversampling:: Oversampling the model. Invoking MakeProfiles * MakeProfiles catalog:: Required catalog properties. * MakeProfiles options:: Full list of MakeProfiles options. * MakeProfiles output:: The generated outputs. MakeNoise * Noise basics:: Noise concepts and definitions. * Invoking astmknoise:: Options and arguments to MakeNoise. Noise basics * Photon counting noise:: Poisson noise * Instrumental noise:: Readout, dark current and other sources. * Final noised pixel value:: How the final noised value is calculated. * Generating random numbers:: How random numbers are generated. High-level calculations * CosmicCalculator:: Calculate cosmological variables CosmicCalculator * Distance on a 2D curved space:: Distances in 2D for simplicity * Extending distance concepts to 3D:: Going to 3D (our real universe). * Invoking astcosmiccal:: How to run CosmicCalculator Libraries * Review of library fundamentals:: Guide on libraries and linking. * Gnuastro library:: Description of all library functions. Review of library fundamentals * Headers:: Header files included in source. * Linking:: Linking the compiled source files into one. * Summary and example on libraries:: A summary and example on using libraries. * Automatic linking script:: Shell function for automatic linking. Gnuastro library * Installation information:: General information about the installation. * Array manipulation:: Functions for manipulating arrays. * Bounding box:: Finding the bounding box. * FITS files:: Working with FITS data. * Git wrappers:: Wrappers for functions in libgit2. * Linked lists:: Various types of linked lists. * Mesh grid for an image:: Breaking an image into a grid. * Polygons:: Working with the vertices of a polygon. * Qsort functions:: Helper functions for Qsort. * Spatial convolution:: Doing spatial convolution on an image * Statistical operations:: Functions for basic statistics. * Multithreaded programming:: Facilitating use of pthreads. * Text table into a C array:: Read an ASCII text table into a C array. * World Coordinate System:: Dealing with the world coordinate system. FITS files (‘fits.h’) * CFITSIO datatype:: Addressing different types of data * FITS macros and data structures:: Gnuastro FITS related macros and structures. * FITS functions:: Functions to work on FITS data. Multithreaded programming (‘threads.h’) * Implementation of pthread_barrier:: Some systems don’t have pthread_barrier * Gnuastro's thread related functions:: Functions for managing threads. Developing * Why C:: Why Gnuastro is designed in C. * Program design philosophy:: General ideas behind the package structure. * Gnuastro project webpage:: Central hub for Gnuastro activities. * Developing mailing lists:: Stay up to date with Gnuastro’s development. * Coding conventions:: Gnuastro coding conventions. * Program source:: Conventions for the code. * Documentation:: Documentation is an integral part of Gnuastro. * Building and debugging:: Build and possibly debug during development. * Test scripts:: Understanding the test scripts. * Developer's checklist:: Checklist to finalize your changes. * Contributing to Gnuastro:: Share your changes with all users. Program source * Mandatory source code files:: Description of files common to all programs. * The TEMPLATE program:: Template for easy creation of a new program. Contributing to Gnuastro * Copyright assignment:: Copyright has to be assigned to the FSF. * Commit guidelines:: Guidelines for commit messages. * Production workflow:: Submitting your commits (work) for inclusion. * Forking tutorial:: Tutorial on workflow steps with Git. Other useful software * SAO ds9:: Viewing FITS images. * PGPLOT:: Plotting directly in C SAO ds9 * Viewing multiextension FITS:: Configure SAO ds9 for multiextension images.  File: gnuastro.info, Node: Introduction, Next: Tutorials, Prev: Top, Up: Top 1 Introduction ************** GNU Astronomy Utilities (Gnuastro) is an official GNU package consisting of separate programs and libraries for the manipulation and analysis of astronomical data. All the programs share the same basic command-line user interface for the comfort of both the users and developers. Gnuastro is written to comply fully with the GNU coding standards so it integrates finely with the GNU/Linux operating system. This also enables astronomers to expect a fully familiar experience in the source code, building, installing and command-line user interaction that they have seen in all the other GNU software that they use. The official and always up to date version of this book (or manual) is freely available under *note GNU Free Documentation License:: in various formats (pdf, html, plain text, info, and as its Texinfo source) at . For users who are new to the GNU/Linux environment, unless otherwise specified most of the topics in *note Installation:: and *note Common program behavior:: are common to all GNU software, for example installation, managing command-line options or getting help (also see *note New to GNU/Linux?::). So if you are new to this empowering environment, we encourage you to go through these chapters carefully. They can be a starting point from which you can continue to learn more from each program’s own manual and fully benefit from and enjoy this wonderful environment. Gnuastro also comes with a large set of libraries, so you can write your own programs using Gnuastro’s building blocks, see *note Review of library fundamentals:: for an introduction. Finally it must be mentioned that in Gnuastro, no change to any program will be released before it has been fully documented in this here first. As discussed in *note Science and its tools:: this is the founding basis of the Gnuastro. * Menu: * Quick start:: A quick start to installation. * Science and its tools:: Some philosophy and history. * Your rights:: User rights. * Naming convention:: About names of programs in Gnuastro. * Version numbering:: Understanding version numbers. * New to GNU/Linux?:: Suggested GNU/Linux distribution. * Report a bug:: Search and report the bug you found. * Suggest new feature:: How to suggest a new feature. * Announcements:: How to stay up to date with Gnuastro. * Conventions:: Conventions used in this book. * Acknowledgments:: People who helped in the production.  File: gnuastro.info, Node: Quick start, Next: Science and its tools, Prev: Introduction, Up: Introduction 1.1 Quick start =============== Gnuastro has three mandatory dependencies and two optional ones for added functionality, see *note Dependencies::. The latest official release tarball is always available as ‘gnuastro-latest.tar.gz’ (http://ftp.gnu.org/gnu/gnuastro/gnuastro-latest.tar.gz). For better compression (faster download), we also provide an Lzip compressed tarball at ‘gnuastro-latest.tar.lz’ (http://ftp.gnu.org/gnu/gnuastro/gnuastro-latest.tar.lz), see *note Release tarball:: for more details on the tarball release. If you have downloaded the tarball in the ‘TOPGNUASTRO’ directory and the dependencies are installed, you can unpack, compile, check and install Gnuastro with the following commands. If you use GNU Tar, the same command (‘$ tar xf’) can also be used to unpack ‘.tar.lz’ tarballs. $ cd TOPGNUASTRO $ tar xf gnuastro-latest.tar.gz # This works on `.tar.lz' too. $ cd gnuastro-X.X # Replace X.X with version number. $ ./configure $ make $ make check $ sudo make install See *note Known issues:: if you confront any complications. For each program there is an ‘Invoke ProgramName’ sub-section in this book which explains how the programs should be run on the command-line. You can read it on the command-line by running the command ‘$ info astprogname’, see *note Naming convention:: and *note Getting help::. The ‘Invoke ProgramName’ sub-section starts with a few examples of each program and goes on to explain the invocation details. In *note Tutorials:: some real life examples of how these programs might be used are given.  File: gnuastro.info, Node: Science and its tools, Next: Your rights, Prev: Quick start, Up: Introduction 1.2 Science and its tools ========================= History of science indicates that there are always inevitably unseen faults, hidden assumptions, simplifications and approximations in all our theoretical models, data acquisition and analysis techniques. It is precisely these that will ultimately allow future generations to advance the existing experimental and theoretical knowledge through their new solutions and corrections. In the past, scientists would gather data and process them individually to achieve an analysis thus having a much more intricate knowledge of the data and analysis. The theoretical models also required little (if any) simulations to compare with the data. Today both methods are becoming increasingly more dependent on pre-written software. Scientists are dissociating themselves from the intricacies of reducing raw observational data in experimentation or from bringing the theoretical models to life in simulations. These ‘intricacies’ are precisely those unseen faults, hidden assumptions, simplifications and approximations that define scientific progress. Unfortunately, most persons who have recourse to a computer for statistical analysis of data are not much interested either in computer programming or in statistical method, being primarily concerned with their own proper business. Hence the common use of library programs and various statistical packages. ... It’s time that was changed. — _F. J. Anscombe. The American Statistician, Vol. 27, No. 1. 1973_ Anscombe’s quartet (1) demonstrates how four data sets with widely different shapes (when plotted) give nearly identical output from standard regression techniques. Anscombe argues that “Good statistical analysis is not a purely routine matter, and generally calls for more than one pass through the computerâ€. Anscombe’s quartet can be generalized to say that users of a software cannot claim to understand how it works only based on the experience they have gained by frequently using it. This kind of subjective experience is prone to very serious mis-understandings about what it really does behind the scenes and can be misleading. This attitude is further encouraged through non-free software(2). This approach to scientific software only helps in producing dogmas and an “obscurantist faith in the expert’s special skill, and in his personal knowledge and authorityâ€(3). Program or be programmed. Choose the former, and you gain access to the control panel of civilization. Choose the latter, and it could be the last real choice you get to make. — _Douglas Rushkoff. Program or be programmed, O/R Books (2010)._ It is obviously impractical for any one human being to gain the intricate knowledge explained above for every step of an analysis. On the other hand, scientific data can be very large and numerous, for example images produced by telescopes in astronomy. This requires very efficient algorithms. To make things worse, natural scientists have generally not been trained in the advanced software techniques, paradigms and architecture that are taught in computer science or engineering courses and thus used in most software. The GNU Astronomy Utilities are an effort to tackle this issue. Gnuastro is not just a software, this book is as important to the idea behind Gnuastro as the source code (software). This book has tried to learn from the success of the “Numerical Recipes†book in educating those who are not software engineers and computer scientists but still heavy users of computational algorithms, like astronomers. There are two major differences: the code and the explanations are segregated: the code is moved within the actual Gnuastro software source code and the underlying explanations are given here. In the source code every non-trivial step is heavily commented and correlated with this book, it follows the same logic of this book, and all the programs follow a similar internal data, function and file structure, see *note Program source::. Complementing the code, this book focuses on thoroughly explaining the concepts behind those codes (history, mathematics, science, software and usage advise when necessary) along with detailed instructions on how to run the programs. At the expense of frustrating “professionals†or “expertsâ€, this book and the comments in the code also intentionally avoid jargon and abbreviations. The source code and this book are thus intimately linked, and when considered as a single entity can be thought of as a real (an actual software accompanying the algorithms) “Numerical Recipes†for astronomy. The other major and arguably more important difference is that “Numerical Recipes†does not allow you to distribute any code that you have learned from it and the book is not freely available. So while it empowers the privileged individual who has access to it, it exacerbates social ignorance. For example it does not allow you to release your software’s source code if you have used their codes, you can only publicly release binaries (a black box) to the community. Exactly at the opposite end of the spectrum, Gnuastro’s source code is released under the GNU general public license (GPL) and this book is released under the GNU free documentation license. You are therefore free to distribute any software you create using parts of Gnuastro’s source code or text, or figures from this book, see *note Your rights::. While developing the source code and this book together, the developers of Gnuastro aim to impose the minimum requirements on you (in computer science, engineering and even the mathematics behind the tools) to understand and modify any step of Gnuastro if you feel the need to do so, see *note Why C:: and *note Program design philosophy::. Imagine if Galileo did not have the technical knowledge to build a telescope. Astronomical objects could not be seen with the Dutch military design of the telescope. In the beginning of his “The Sidereal Messenger†(1610) he cautions the readers on this issue and instructs them on how to build a suitable instrument: without a detailed description of “how†he made his observations, no one would believe him. The same is true today, science cannot progress with a black box. Before he actually saw the moons of Jupiter, the mountains on the Moon or the crescent of Venus, he was an anti-Copernican and was “evasive†to Kepler(4). Science is not independent of its tools. Bjarne Stroustrup (creator of the C++ language) says: “Without understanding software, you are reduced to believing in magicâ€. Ken Thomson (the designer or the Unix operating system) says “I abhor a system designed for the ‘user’ if that word is a coded pejorative meaning ‘stupid and unsophisticated’.†Certainly no scientist (user of a scientific software) would want to be considered a believer in magic, or ‘stupid and unsophisticated’. However, this can happen when scientists get too distant from the raw data and are mainly indulging themselves in their own high-level (abstract) models (creations). For example, roughly 5 years before special relativity and about two decades before quantum mechanics fundamentally changed Physics, Kelvin is quoted as saying: There is nothing new to be discovered in physics now. All that remains is more and more precise measurement. — _William Thomson (Lord Kelvin), 1900_ A few years earlier, in a speech Albert. A. Michelson said: The more important fundamental laws and facts of physical science have all been discovered, and these are now so firmly established that the possibility of their ever being supplanted in consequence of new discoveries is exceedingly remote.... Our future discoveries must be looked for in the sixth place of decimals. — _Albert. A. Michelson, dedication of Ryerson Physics Lab, U. Chicago 1894_ If scientists are considered to be more than mere “puzzle solversâ€(5) (simply adding to the decimals of known values or observing a feature in 10, 100, or 100000 more galaxies or stars, as Kelvin and Michelson clearly believed), they cannot just passively sit back and uncritically repeat the previous (observational or theoretical) methods/tools on new data. Today there is a wealth of raw telescope images ready (mostly for free) at the finger tips of anyone who is interested with a fast enough internet connection to download them. The only thing lacking is new ways to analyze this data and dig out the treasure that is lying hidden in them to existing methods and techniques. New data that we insist on analyzing in terms of old ideas (that is, old models which are not questioned) cannot lead us out of the old ideas. However many data we record and analyze, we may just keep repeating the same old errors, missing the same crucially important things that the experiment was competent to find. — _E. T. Jaynes, Probability theory, the logic of science. 2003._ ---------- Footnotes ---------- (1) (2) (3) Karl Popper. The logic of scientific discovery. 1959. Larger quote is given at the start of the PDF (for print) version of this book. (4) Galileo G. (Translated by Maurice A. Finocchiaro). _The essential Galileo_. Hackett publishing company, first edition, 2008. (5) Thomas S. Kuhn. _The Structure of Scientific Revolutions_, University of Chicago Press, 1962.  File: gnuastro.info, Node: Your rights, Next: Naming convention, Prev: Science and its tools, Up: Introduction 1.3 Your rights =============== The paragraphs below, in this section, belong to the GNU Texinfo(1) manual and are not written by us! The name “Texinfo†is just changed to “GNU Astronomy Utilities†or “Gnuastro†because they are released under the same licenses and it is beautifully written to inform you of your rights. GNU Astronomy Utilities is “free softwareâ€; this means that everyone is free to use it and free to redistribute it on certain conditions. Gnuastro is not in the public domain; it is copyrighted and there are restrictions on its distribution, but these restrictions are designed to permit everything that a good cooperating citizen would want to do. What is not allowed is to try to prevent others from further sharing any version of Gnuastro that they might get from you. Specifically, we want to make sure that you have the right to give away copies of the programs that relate to Gnuastro, that you receive the source code or else can get it if you want it, that you can change these programs or use pieces of them in new free programs, and that you know you can do these things. To make sure that everyone has such rights, we have to forbid you to deprive anyone else of these rights. For example, if you distribute copies of the Gnuastro related programs, you must give the recipients all the rights that you have. You must make sure that they, too, receive or can get the source code. And you must tell them their rights. Also, for our own protection, we must make certain that everyone finds out that there is no warranty for the programs that relate to Gnuastro. If these programs are modified by someone else and passed on, we want their recipients to know that what they have is not what we distributed, so that any problems introduced by others will not reflect on our reputation. The precise conditions of the licenses for the programs currently being distributed that relate to Gnuastro are found in the GNU General Public license (http://www.gnu.org/copyleft/gpl.html) that accompany them. This book is covered by the GNU Free Documentation License (http://www.gnu.org/copyleft/fdl.html). ---------- Footnotes ---------- (1) Texinfo is the GNU documentation system. It is used to create this book in all the various formats.  File: gnuastro.info, Node: Naming convention, Next: Version numbering, Prev: Your rights, Up: Introduction 1.4 Naming convention ===================== Gnuastro is a package of independent programs and a collection of libraries, here we are mainly concerned with the programs. Each program has an official name which consists of one or two words, describing what they do. The latter are printed with no space, for example NoiseChisel or ImageCrop. On the command-line, you can run them with their executable names which start with an ‘ast’ and might be an abbreviation of the official name, for example ‘astnoisechisel’ or ‘astimgcrop’, see *note Executable names::. We will use “ProgramName†for a generic official program name and ‘astprogname’ for a generic executable name. In this book, the programs are classified based on what they do and thoroughly explained. An alphabetical list of the programs that are installed on your system with this installation are given in *note Gnuastro programs list::. That list also contains the executable names and version numbers along with a one line description.  File: gnuastro.info, Node: Version numbering, Next: New to GNU/Linux?, Prev: Naming convention, Up: Introduction 1.5 Version numbering ===================== Gnuastro can have two formats of version numbers, for official and unofficial releases. Official Gnuastro releases are announced on the ‘info-gnuastro’ mailing list, they have a version control tag in Gnuastro’s development history, and their version numbers are formatted like “‘A.B’â€. ‘A’ is a major version number, marking a significant planned achievement (for example see *note GNU Astronomy Utilities 1.0::), while ‘B’ is a minor version number, see below for more on the distinction. Note that the numbers are not decimals, so version 2.34 is much more recent than version 2.5, which is not equal to 2.50. Gnuastro also allows a unique version number for unofficial releases. Unofficial releases can mark any point in Gnuastro’s development history. This is done to allow astronomers to easily use any point in the version controlled history for their data-analysis and research publication. See *note Version controlled source:: for a complete introduction. This section is not just for developers and is very straightforward, so please have a look if you are interested in the cutting-edge. This unofficial version number is a meaningful and easy to read string of characters, unique to that particular point of history. With this feature, users can easily stay up to date with the most recent bug fixes and additions that are committed between official releases. The unofficial version number is formatted like: ‘A.B.C-D’. ‘A’ and ‘B’ are the most recent official version number. ‘C’ is the number of commits that have been made after version ‘A.B’. ‘D’ is the first 4 or 5 characters of the commit hash number(1). Therefore, the unofficial version number ‘‘3.92.8-29c8’’, corresponds to the 8th commit after the official version ‘3.92’ and its commit hash begins with ‘29c8’. The unofficial version number is sort-able (unlike the raw hash) and as shown above is very descriptive of the state of the unofficial release. Of course an official release is preferred for publication (since its tarballs are easily available and it has gone through more tests, making it more stable), so if an official release is announced prior to your publication’s final review, please consider updating to the official release. The major version number is set by a major goal which is defined by the developers and user community before hand, for example see *note GNU Astronomy Utilities 1.0::. The incremental work done in minor releases are commonly small steps in achieving the major goal. Therefore, there is no limit on the number of minor releases and the difference between the (hypothetical) versions 2.927 and 3.0 can be a very small (negligible to the user) improvement that finalizes the defined goals. * Menu: * GNU Astronomy Utilities 1.0:: Plans for version 1.0 release ---------- Footnotes ---------- (1) Each point in Gnuastro’s history is uniquely identified with a 40 character long hash which is created from its contents and previous history for example: ‘5b17501d8f29ba3cd610673261e6e2229c846d35’. So the string ‘D’ in the version for this commit could be ‘5b17’, or ‘5b175’.  File: gnuastro.info, Node: GNU Astronomy Utilities 1.0, Prev: Version numbering, Up: Version numbering 1.5.1 GNU Astronomy Utilities 1.0 --------------------------------- Currently (prior to Gnuastro 1.0), the aim of Gnuastro is to have a complete system for data manipulation and analysis at least similar to IRAF(1). So an astronomer can take all the standard data analysis steps (starting from raw data to the final reduced product and standard post-reduction tools) with the various programs in Gnuastro. The maintainers of each camera or detector on a telescope can provide a completely transparent shell script or Makefile to the observer for data analysis. This script can set configuration files for all the required programs to work with that particular camera. The script can then run the proper programs in the proper sequence. The user/observer can easily follow the standard shell script to understand (and modify) each step and the parameters used easily. Bash (or other modern GNU/Linux shell scripts) are very powerful and made for this gluing job. This will simultaneously improve performance and transparency. Shell scripting (or Makefiles) are also very basic constructs that are easy to learn and readily available as part of the Unix-like operating systems. If there is no program to do a desired step, Gnuastro’s libraries can be used to build specific programs. The main factor is that all observatories or projects can freely contribute to Gnuastro and all simultaneously benefit from it (since it doesn’t belong to any particular one of them), much like how for-profit organizations (for example RedHat, or Intel and many others) are major contributors to free and open source software for their shared benefit. Gnuastro’s copyright has been fully awarded to GNU, so it doesn’t belong to any particular astronomer or astronomical facility or project. ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: New to GNU/Linux?, Next: Report a bug, Prev: Version numbering, Up: Introduction 1.6 New to GNU/Linux? ===================== Some astronomers initially install and use the GNU/Linux operating systems because the software that their research community use can only be run in this environment, the transition is not necessarily easy. To encourage you in investing the patience and time to make this transition, we define the GNU/Linux system and argue for the command-line interface of scientific software and how it is worth the (apparently steep) learning curve. *note Command-line interface:: contains a short overview of the very powerful command-line user interface. *note Tutorials:: is a complete chapter with some real world example applications of Gnuastro making good use of GNU/Linux capabilities written for newcomers to this environment. It is fully explained, easy and (hopefully) entertaining. You might have already noticed that we are not using the name “Linuxâ€, but “GNU/Linuxâ€. Please take the time to have a look at the following essays and FAQs for a complete understanding of this very important distinction. In short, the Linux kernel is built using the GNU C library (glibc) and GNU compiler collection (gcc). The Linux kernel software alone is useless, in order have an operating system you need many more packages and the majority of such low-level packages in most distributions are developed as part of the GNU project: “the whole system is basically GNU with Linux loadedâ€. In the form of an analogy: to say “running Linuxâ€, is like saying “driving your carburetorâ€. • • • • * Menu: * Command-line interface:: Introduction to the command-line  File: gnuastro.info, Node: Command-line interface, Prev: New to GNU/Linux?, Up: New to GNU/Linux? 1.6.1 Command-line interface ---------------------------- One aspect of Gnuastro that might be a little troubling to new GNU/Linux users is that (at least for the time being) it only has a command-line user interface (CLI). This might be contrary to the mostly graphical user interface (GUI) experience with proprietary operating systems. To a first time user, the command-line does appear much more complicated and adapting to it might not be easy and a little frustrating at first. This is understandable and also experienced by anyone who started using the computer (from childhood) in a graphical user interface. Here we hope to convince you of the unique benefits of this interface which can greatly enhance your productivity while complementing your GUI experience. Through GNOME 3(1), most GNU/Linux based operating systems now have a very advanced and useful GUI. Since the GUI was created long after the command-line, some wrongly consider the command line to be obsolete. Both interfaces are very useful for different tasks (for example you can’t view an image, video, pdf document or web page on the command-line!), on the other hand you can’t reproduce your results easily in the GUI. Therefore they should not be regarded as rivals but as complementary user interfaces, here we will outline how the CLI can be useful in scientific programs. You can think of the GUI as a veneer over the CLI to facilitate a small subset of all the possible CLI operations. Each click you do on the GUI, can be thought of as internally running a different CLI command. So asymptotically (if a good designer can design a GUI which is able to show you all the possibilities to click on) the GUI is only as powerful as the command-line. In practice, such graphical designers are very hard to find for every program, so the GUI operations are always a subset of the internal CLI commands. For programs that are only made for the GUI, this results in not including lots of potentially useful operations. It also results in ‘interface design’ to be a crucially important part of any GUI program. Scientists don’t usually have enough resources to hire a graphical designer, also the complexity of the GUI code is far more than CLI code, which is harmful for a scientific software, see *note Science and its tools::. For programs that have a GUI, one action on the GUI (moving and clicking a mouse, or tapping a touchscreen) might be more efficient and easier than its CLI counterpart (typing the program name and your desired configuration). However, if you have to repeat that same action more than once, the GUI will soon become very frustrating and prone to errors. Unless the designers of a particular program decided to design such a system for a particular GUI action, there is no general way to run any possible series of actions automatically on the GUI. On the command-line, you can run any series of of actions which can come from various CLI capable programs you have decided your self in any possible permutation with one command(2). This allows for much more creativity and exact reproducibility that is not possible to a GUI user. For technical and scientific operations, where the same operation (using various programs) has to be done on a large set of data files, this is crucially important. It also allows exact reproducibility which is a foundation principle for scientific results. The most common CLI (which is also known as a shell) in GNU/Linux is GNU Bash, we strongly encourage you to put aside several hours and go through this beautifully explained web page: . You don’t need to read or even fully understand the whole thing, only a general knowledge of the first few chapters are enough to get you going. Since the operations in the GUI are very limited and they are visible, reading a manual is not that important in the GUI (most programs don’t even have any!). However, to give you the creative power explained above, with a CLI program, it is best if you first read the manual of any program you are using. You don’t need to memorize any details, only an understanding of the generalities is needed. Once you start working, there are more easier ways to remember a particular option or operation detail, see *note Getting help::. To experience the command-line in its full glory and not in the GUI terminal emulator, press the following keys together: (3) to access the virtual console. To return back to your GUI, press the same keys above replacing with (or , or , depending on your GNU/Linux distribution). In the virtual console, the GUI, with all its distracting colors and information, is gone. Enabling you to focus entirely on your actual work. For operations that use a lot of your system’s resources (processing a large number of large astronomical images for example), the virtual console is the place to run them. This is because the GUI is not competing with your research work for your system’s RAM and CPU. Since the virtual consoles are completely independent, you can even log out of your GUI environment to give even more of your hardware resources to the programs you are running and thus reduce the operating time. Since it uses far less system resources, the CLI is also very convenient for remote access to your computer. Using secure shell (SSH) you can log in securely to your system (similar to the virtual console) from anywhere even if the connection speeds are low. There are apps for smart phones and tablets which allow you to do this. ---------- Footnotes ---------- (1) (2) By writing a shell script and running it, for example see the tutorials in *note Tutorials::. (3) Instead of , you can use any of the keys from to for different virtual consoles depending on your GNU/Linux distribution, try them all out. You can also run a separate GUI from within this console if you want to.  File: gnuastro.info, Node: Report a bug, Next: Suggest new feature, Prev: New to GNU/Linux?, Up: Introduction 1.7 Report a bug ================ According to Wikipedia “a software bug is an error, flaw, failure, or fault in a computer program or system that causes it to produce an incorrect or unexpected result, or to behave in unintended waysâ€. So when you see that a program is crashing, not reading your input correctly, giving the wrong results, or not writing your output correctly, you have found a bug. In such cases, it is best if you report the bug to the developers. The programs will also report bugs in known impossible situations (which are caused by something unexpected) and will ask the users to report the bug. Prior to actually filing a bug report, it is best to search previous reports. The issue might have already been found and even solved. The best place to check if your bug has already been discussed is the bugs tracker on *note Gnuastro project webpage:: at . In the top search fields (under “Display Criteriaâ€) set the “Open/Closed†drop-down menu to “Any†and choose the respective program or general category of the bug in “Category†and click the “Apply†button. The results colored green have already been solved and the status of those colored in red is shown in the table. Recently corrected bugs are probably not yet publicly released because they are scheduled for the next Gnuastro stable release. If the bug is solved but not yet released and it is an urgent issue for you, you can get the version controlled source and compile that, see *note Version controlled source::. To solve the issue as readily as possible, please follow the following to guidelines in your bug report. The How to Report Bugs Effectively (http://www.chiark.greenend.org.uk/~sgtatham/bugs.html) and How To Ask Questions The Smart Way (http://catb.org/~esr/faqs/smart-questions.html) essays also provide some very good generic advice for all software (don’t contact their authors for Gnuastro’s problems). Mastering the art of giving good bug reports (like asking good questions) can greatly enhance your experience with any free and open source software. So investing the time to read through these essays will greatly reduce your frustration after you see something doesn’t work the way you feel it is supposed to for a large range of software, not just Gnuastro. *Be descriptive* Please provide as many details as possible and be very descriptive. Explain what you expected and what the output was: it might be that your expectation was wrong. Also please clearly state which sections of the Gnuastro book (this book), or other references you have studied to understand the problem. This can be useful in correcting the book (adding links to likely places where users will check). But more importantly, it will be very encouraging for the developers, since you are showing how serious you are about the problem and that you have actually put some thought into it. “To be able to ask a question clearly is two-thirds of the way to getting it answered.†– John Ruskin (1819-1900). *Individual and independent bug reports* If you have found multiple bugs, please send them as separate (and independent) bugs (as much as possible). This will significantly help us in managing and resolving them sooner. *Reproducible bug reports* If we cannot exactly reproduce your bug, then it is very hard to resolve it. So please send us a Minimal working example(1) along with the description. For example in running a program, please send us the full command-line text and the output with the ‘-P’ option, see *note Final parameter values::. If it is caused only for a certain input, also send us that input file. In case the input FITS is large, please use ImageCrop to only crop the problematic section and make it as small as possible so it can easily be uploaded and downloaded and not waste the archive’s storage, see *note ImageCrop::. There are generally two ways to inform us of bugs: • Send a mail to ‘bug-gnuastro@gnu.org’. Any mail you send to this address will be distributed through the bug-gnuastro mailing list(2). This is the simplest way to send us bug reports. The developers will then register the bug into the project webpage (next choice) for you. • Use the Gnuastro project webpage at : There are two ways to get to the submission page as listed below. Fill in the form as described below and submit it (see *note Gnuastro project webpage:: for more on the project webpage). • Using the top horizontal menu items, immediately under the top page title. Hovering your mouse on “Support†will open a drop-down list. Select “Submit newâ€. • In the main body of the page, under the “Communication tools†section, click on “Submit new itemâ€. Once the items have been registered in the mailing list or webpage, the developers will add it to either the “Bug Tracker†or “Task Manager†trackers of the Gnuastro project webpage. These two trackers can only be edited by the Gnuastro project developers, but they can be browsed by anyone, so you can follow the progress on your bug. You are most welcome to join us in developing Gnuastro and fixing the bug you have found maybe a good starting point. Gnuastro is designed to be easy for anyone to develop (see *note Science and its tools::) and there is a full chapter devoted to developing it: *note Developing::. ---------- Footnotes ---------- (1) (2)  File: gnuastro.info, Node: Suggest new feature, Next: Announcements, Prev: Report a bug, Up: Introduction 1.8 Suggest new feature ======================= We would always be very happy to hear of suggested new features. For every program there are already lists of features that we are planning to add. You can see the current list of plans from the Gnuastro project webpage at and following “Tasksâ€â†’“Browse†on the horizontal menu at the top of the page immediately under the title, see *note Gnuastro project webpage::. If you want to request a feature to an existing program, click on the “Display Criteria†above the list and under “Categoryâ€, choose that particular program. Under “Category†you can also see the existing suggestions for new programs or other cases like installation, documentation or libraries. Also be sure to set the “Open/Closed†value to “Anyâ€. If the feature you want to suggest is not already listed in the task manager, then follow the steps that are fully described in *note Report a bug::. Please have in mind that the developers are all very busy with their own astronomical research, and implementing existing “taskâ€s to add or resolving bugs. Gnuastro is a volunteer effort and none of the developers are paid for their hard work. So, although we will try our best, please don’t not expect that your suggested feature be immediately included (with the next release of Gnuastro). The best person to apply the exciting new feature you have in mind is you, since you have the motivation and need. In fact Gnuastro is designed for making it as easy as possible for you to hack into it (add new features, change existing ones and so on), see *note Science and its tools::. Please have a look at the chapter devoted to developing (*note Developing::) and start applying your desired feature. Once you have added it, you can use it for your own work and if you feel you want others to benefit from your work, you can request for it to become part of Gnuastro. You can then join the developers and start maintaining your own part of Gnuastro. If you choose to take this path of action please contact us before hand (*note Report a bug::) so we can avoid possible duplicate activities and get interested people in contact. *Gnuastro is a collection of low level programs:* As described in *note Program design philosophy::, a founding principle of Gnuastro is that each library or program should be very basic and low-level. High level jobs should be done by running the separate programs or using separate functions in succession through a shell script or calling the libraries by higher level functions, see the examples in *note Tutorials::. So when making the suggestions please consider how your desired job can best be broken into separate steps and modularized.  File: gnuastro.info, Node: Announcements, Next: Conventions, Prev: Suggest new feature, Up: Introduction 1.9 Announcements ================= Gnuastro has a dedicated mailing list for making announcements. Anyone that is interested can subscribe to this mailing list to stay up to date with new releases or when the dependencies (see *note Dependencies::) have been updated. To subscribe to this list, please visit .  File: gnuastro.info, Node: Conventions, Next: Acknowledgments, Prev: Announcements, Up: Introduction 1.10 Conventions ================ In this book we have the following conventions: • All commands that are to be run on the shell (command-line) prompt as the user start with a ‘$’. In case they must be run as a super-user or system administrator, they will start with a ‘#’. If the command is in a separate line and next line ‘is also in the code type face’, but doesn’t have any of the ‘$’ or ‘#’ signs, then it is the output of the command after it is run. As a user, you don’t need to type those lines. • If the command becomes larger than the page width a <\> is inserted in the code. If you are typing the code by hand on the command-line, you don’t need to use multiple lines or add the extra space characters, so you can omit them. If you want to copy and paste these examples (highly discouraged!) then the <\> should stay. The <\> character is a shell escape character which is used commonly to make characters which have special meaning for the shell loose that special place (the shell will not treat them specially if there is a <\> behind them). When it is a last character in a line (the next character is a new-line character) the new-line character looses its meaning an the shell sees it as a simple white-space character, enabling you to use multiple lines to write your commands.  File: gnuastro.info, Node: Acknowledgments, Prev: Conventions, Up: Introduction 1.11 Acknowledgments ==================== The list of Gnuastro authors is available at the start of this book and the ‘AUTHORS’ file in the source code. Here the authors wish to gratefully acknowledge the help and support they received from other people and institutions who had an indirect (not committed in the version controlled history) role in Gnuastro. The plain text file ‘THANKS’ which is distributed along with the source code also contains this list. The Japanese Ministry of Science and Technology (MEXT) scholarship for Mohammad Akhlaghi’s Masters and PhD period in Tohoku University Astronomical Institute had an instrumental role in the long term learning and planning that made the idea of Gnuastro possible. The very critical view points of Professor Takashi Ichikawa (from Tohoku University) were also instrumental in the initial ideas and creation of Gnuastro. Brandon Invergo, Karl Berry and Richard Stallman also provided very useful suggestions during the GNU evaluation process. Bob Proulx from Savannah, has kindly supported Gnuastro’s project webpage on Savannah and the management of its version controlled source server there. We would also like to gratefully thank Mohammad-reza Khellat, Alan Lefor, Yahya Sefidbakht, Francesco Montanari, and Ole Streicher for their useful and constructive comments and suggestions. Finally we should thank all the (sometimes anonymous) developers in various online forums which patiently answered all our small (but important) technical questions. All work on Gnuastro has been voluntary, but we are most grateful to the following institutions (in chronological order) for hosting us in our research: Ministry of education, culture, sports, science and technology (MEXT), Japan. Tohoku University Astronomical Institute, Sendai, Japan. University of Salento, Lecce, Italy. Centre national de la recherche scientifique (CNRS), France. Centre de Recherche Astrophysique de Lyon, University of Lyon 1, France.  File: gnuastro.info, Node: Tutorials, Next: Installation, Prev: Introduction, Up: Top 2 Tutorials *********** In this chapter we give several tutorials or cookbooks on how to use the various tools in Gnuastro for your scientific purposes. In these tutorials, we have intentionally avoided too many cross references to make it more easily readable. To get more information about a particular program, you can visit the section with the same name as the program in this book. Each program section starts by explaining the general concepts behind what it does. If you only want to see an explanation of the options and arguments of any program, see the subsection titled ‘Invoking ProgramName’. See *note Conventions::, for an explanation of the conventions we use in the example codes through the book. The tutorials in this section use a fictional setting of some historical figures in the history of astronomy. We have tried to show how Gnuastro would have been helpful for them in making their discoveries if there were GNU/Linux computers in their times! Please excuse us for any historical inaccuracy, this is not intended to be a historical reference. This form of presentation can make the tutorials more pleasant and entertaining to read while also being more practical (explaining from a user’s point of view)(1). The main reference for the historical facts mentioned in these fictional settings was Wikipedia. * Menu: * Hubble visually checks and classifies his catalog:: Check a catalog. * Sufi simulates a detection:: Simulating a detection. ---------- Footnotes ---------- (1) This form of presenting a tutorial was influenced by the PGF/TikZ and Beamer manuals. The first provides graphic capabilities, while with the second you can make presentation slides in TeX and LaTeX. In these manuals, Till Tantau (author of the manual) uses Euclid as the protagonist. There are also some nice words of wisdom for Unix-like systems called “Rootless Rootâ€: . These also have a similar style but they use a mythical figure named Master Foo. If you already have some experience in Unix-like systems, you will definitely find these “Unix Koans†very entertaining.  File: gnuastro.info, Node: Hubble visually checks and classifies his catalog, Next: Sufi simulates a detection, Prev: Tutorials, Up: Tutorials 2.1 Hubble visually checks and classifies his catalog ===================================================== In 1924 Hubble(1) announced his discovery that some of the known nebulous objects are too distant to be within the the Milky Way (or Galaxy) and that they were probably distant Galaxies(2) in their own right. He had also used them to show that the redshift of the nebulae increases with their distance. So now he wants to study them more accurately to see what they actually are. Since they are nebulous or amorphous, they can’t be modeled (like stars that are always a point) easily. So there is no better way to distinguish them than to visually inspect them and see if it is possible to classify these nebulae or not. Hubble has stored all the FITS images of the objects he wants to visually inspect in his ‘/mnt/data/images’ directory. He has also stored his catalog of extra Galactic nebulae in ‘/mnt/data/catalogs/extragalactic.txt’. Any normal user on his GNU/Linux system (including himself) only has read access to the contents of the ‘/mnt/data’ directory. He has done this by running this command as root: # chmod -R 755 /mnt/data Hubble has done this intentionally to avoid mistakenly deleting or modifying the valuable images he has taken at Mount Wilson while he is working as an ordinary user. Retaking all those images and data is simply not an option. In fact they are also in another hard disk (‘/dev/sdb1’). So if the hard disk which stores his GNU/Linux distribution suddenly malfunctions due to work load, his data is not in harms way. That hard disk is only mounted to this directory when he wants to use it with the command: # mount /dev/sdb1 /mnt/data In short, Hubble wants to keep his data safe and fortunately by default Gnuastro allows for this. Hubble creates a temporary ‘visualcheck’ directory in his home directory for this check. He runs the following commands to make the directory and change to it(3): $ mkdir ~/visualcheck $ cd ~/visualcheck $ pwd /home/edwin/visualcheck $ ls Hubble has multiple images in ‘/mnt/data/images’, some of his targets might be on the edges of an image and so several images need to be stitched to give a good view of them. Also his extra Galactic targets belong to various pointings in the sky, so they are not in one large image. Gnuastro’s ImageCrop is just the program he wants. The catalog in ‘extragalactic.txt’ is a plain text file which stores the basic information of all his known 200 extra Galactic nebulae. In its second column it has each object’s Right Ascension (the first column is a label he has given to each object) and in the third the object’s declination. Having read the Gnuastro manual, he knows that all counting is done starting from zero, so the RA and Dec columns have number 1 and 2 respectively. $ astimgcrop --racol=1 --deccol=2 /mnt/data/images/*.fits \ /mnt/data/catalogs/extragalactic.txt ImageCrop started on Tue Jun 14 10:18:11 1932 ---- ./4_crop.fits 1 1 ---- ./2_crop.fits 1 1 ---- ./1_crop.fits 1 1 [[[ Truncated middle of list ]]] ---- ./198_crop.fits 1 1 ---- ./195_crop.fits 1 1 - 200 images created. - 200 were filled in the center. - 0 used more than one input. ImageCrop finished in: 2.429401 (seconds) Hubble already knows that thread allocation to the the CPU cores is asynchronous, so each time you run it the order of which job gets done first differs. When using ImageCrop the order of outputs is irrelevant since each crop is independent of the rest. This is why the crops are not necessarily created in the same input order. He is content with the default width of the outputs (which he inspected by running ‘$ astimgcrop -P’). If he wanted a different width for the cropped images, he could do that with the ‘--wwidth’ option which accepts a value in arc-seconds. When he lists the contents of the directory again he finds his 200 objects as separate FITS images. $ ls 1_crop.fits 2_crop.fits ... 200_crop.fits The FITS image format was not designed for viewing, but mainly for accurate storing of the data. So he chooses to convert the cropped images to a more common image format to view them more quickly and easily through standard image viewers (which load much faster than FITS image viewer). JPEG is one of the most recognized image formats that is supported by most image viewers. Fortunately Gnuastro has just such a tool to convert various types of file types to and from each other: ConvertType. Hubble has already heard of GNU Parallel from one of his colleagues at Mount Wilson Observatory. It allows multiple instances of a command to be run simultaneously on the system, so he uses it in conjunction with ConvertType to convert all the images to JPEG. $ parallel astconvertt -ojpg ::: *_crop.fits For his graphical user interface Hubble is using GNOME which is the default in most distributions in GNU/Linux. The basic image viewer in GNOME is the Eye of GNOME, which has the executable file name ‘eog’ (4). Since he has used it before, he knows that once it opens an image, he can use the or keys on the keyboard to go to the next image in the directory or the key to to go the previous image. So he opens the image of the first object with the command below and with his cup of coffee in his other hand, he flips through his targets very fast to get a good initial impression of the morphologies of these extra Galactic nebulae. $ eog 1_crop.jpg Hubble’s cup of coffee is now finished and he also got a nice general impression of the shapes of the nebulae. He tentatively/mentally classified the objects into three classes while doing the visual inspection. One group of the nebulae have a very simple elliptical shape and seem to have no internal special structure, so he gives them code 1. Another clearly different class are those which have spiral arms which he associates with code 2 and finally there seems to be a class of nebulae in between which appear to have a disk but no spiral arms, he gives them code 3. Now he wants to know how many of the nebulae in his extra Galactic sample are within each class. Repeating the same process above and writing the results on paper is very time consuming and prone to errors. Fortunately Hubble knows the basics of GNU Bash shell programming, so he writes the following short script with a loop to help him with the job. After all, computers are made for us to operate and knowing basic shell programming gives Hubble this ability to creatively operate the computer as he wants. So using GNU Emacs(5) (his favorite text editor) he puts the following text in a file named ‘classify.sh’. for name in *.jpg do eog $name & processid=$! echo -n "$name belongs to class: " read class echo $name $class >> classified.txt kill $processid done Fortunately GNU Emacs or even simpler editors like Gedit (part of the GNOME graphical user interface) will display the variables and shell constructs in different colors which can really help in understanding the script. Put simply, the ‘for’ loop gets the name of each JPEG file in the directory this script is run in and puts it in ‘name’. In the shell, the value of a variable is used by putting a ‘$’ sign before the variable name. Then Eye of GNOME is run on the image in the background to show him that image and its process ID is saved internally (this is necessary to close Eye of GNOME later). The shell then prompts the user to specify a class and after saving it in ‘class’, it prints the file name and the given class in the next line of a file named ‘classified.txt’. To make the script executable (so he can run it later any time he wants) he runs: $ chmod +x classify.sh Now he is ready to do the classification, so he runs the script: $ ./classify.sh In the end he can delete all the JPEG and FITS files along with ImageCrop’s log file with the following short command. The only files remaining are the script and the result of the classification. $ rm *.jpg *.fits astimgcrop.txt $ ls classified.txt classify.sh He can now use ‘classified.txt’ as input to a plotting program to plot the histogram of the classes and start making interpretations about what these nebulous objects that are outside of the Galaxy are. ---------- Footnotes ---------- (1) Edwin Powell Hubble (1889 – 1953 A.D.) was an American astronomer who can be considered as the father of extra-galactic astronomy, by proving that some nebulae are too distant to be within the Galaxy. He then went on to show that the universe appears to expand and also done a visual classification of the galaxies that is known as the Hubble fork. (2) Note that at that time, “Galaxy†was a proper noun used to refer to the Milky way. The concept of a galaxy as we define it today had not yet become common. Hubble played a major role in creating today’s concept of a galaxy. (3) The ‘pwd’ command is short for “Print Working Directory†and ‘ls’ is short for “list†which shows the contents of a directory. (4) Eye of GNOME is only available for users of the GNOME graphical desktop environment which is the default in most GNU/Linux distributions. If you use another graphical desktop environment, replace ‘eog’ with any other image viewer. (5) This can be done with any text editor  File: gnuastro.info, Node: Sufi simulates a detection, Prev: Hubble visually checks and classifies his catalog, Up: Tutorials 2.2 Sufi simulates a detection ============================== It is the year 953 A.D. and Sufi(1) is in Shiraz as a guest astronomer. He had come there to use the advanced 123 centimeter astrolabe for his studies on the Ecliptic. However, something was bothering him for a long time. While mapping the constellations, there were several non-stellar objects that he had detected in the sky, one of them was in the Andromeda constellation. During a trip he had to Yemen, Sufi had seen another such object in the southern skies looking over the Indian ocean. He wasn’t sure if such cloud-like non-stellar objects (which he was the first to call ‘SahÄbi’ in Arabic or ‘nebulous’) were real astronomical objects or if they were only the result of some bias in his observations. Could such diffuse objects actually be detected at all with his detection technique? He still had a few hours left until nightfall (when he would continue his studies on the ecliptic) so he decided to find an answer to this question. He had thoroughly studied Claudius Ptolemy’s (90 – 168 A.D) Almagest and had made lots of corrections to it, in particular in measuring the brightness. Using his same experience, he was able to measure a magnitude for the objects and wanted to simulate his observation to see if a simulated object with the same brightness and size could be detected in a simulated noise with the same detection technique. The general outline of the steps he wants to take are: 1. Make some mock profiles in an oversampled image. The initial mock image has to be oversampled prior to convolution or other forms of transformation in the image. Through his experiences, Sufi knew that this is because the image of heavenly bodies is actually transformed by the atmosphere or other sources outside the atmosphere (for example gravitational lenses) prior to being sampled on an image. Since that transformation occurs on a continuous grid, to best approximate it, he should do all the work on a finer pixel grid. In the end he can re-sample the result to the initially desired grid size. 2. Convolve the image with a PSF image that is oversampled to the same value as the mock image. Since he wants to finish in a reasonable time and the PSF kernel will be very large due to oversampling, he has to use frequency domain convolution which has the side effect of dimming the edges of the image. So in the first step above he also has to build the image to be larger by at least half the width of the PSF convolution kernel on each edge. 3. With all the transformations complete, the image should be re-sampled to the same size of the pixels in his detector. 4. He should remove those extra pixels on all edges to remove frequency domain convolution artifacts in the final product. 5. He should add noise to the (until now, noise-less) mock image. After all, all observations have noise associated with them. Fortunately Sufi had heard of GNU Astronomy Utilities from a colleague in Isfahan (where he worked) and had installed it on his computer a year before. It had tools to do all the steps above. He had used MakeProfiles before, but wasn’t sure which columns he had chosen in his user or system wide configuration files for which parameters, see *note Configuration files::. So to start his simulation, Sufi runs MakeProfiles with the ‘-P’ option to make sure what columns in a catalog MakeProfiles currently recognizes and the output image parameters: $ astmkprof -P # MakeProfiles (GNU Astronomy Utilities 0.1) 0.1 # Configured on 21 September 952 at 19:37 # Written on Sat Oct 6 15:49:31 953 # Output: naxis1 1000 naxis2 1000 oversample 5 [[[ Truncated middle of list ]]] # Catalog: xcol 1 ycol 2 fcol 3 rcol 4 ncol 5 pcol 6 qcol 7 mcol 8 tcol 9 [[[ Truncated rest of list ]]] In particular, Sufi looks at the parameters under the catalog grouping. Fortunately the columns are naturally numbered such that column 0 can be an ID he specifies for each object (which MakeProfiles ignores) and each subsequent column specifies a given parameter. Fortunately MakeProfiles has the capability to also make the PSF which is to be used on the mock image and using the ‘--prepforconv’ option, he can also make the mock image to be larger by the correct amount and all the sources to be shifted by the correct amount. For his initial check he decides to simulate the nebula in the Andromeda constellation. The night he was observing, the PSF had roughly a FWHM of about 5 pixels, so as the first row, he defines the PSF parameters and sets the radius column (‘rcol’ above, fifth column) to ‘5.000’, he also chooses a Moffat function for its functional form. Remembering how diffuse the nebula in the Andromeda constellation was, he decides to simulate it with a mock Sérsic index 1.0 profile. He wants the output to be 500 pixels by 500 pixels, so he puts the mock profile in the center. Looking at his drawings of it, he decides a reasonable effective radius for it would be 40 pixels on this image pixel scale, he sets the axis ratio and position angle to approximately correct values too and finally he sets the total magnitude of the profile to 3.44 which he had accurately measured. Sufi also decides to truncate both the mock profile and PSF at 5 times the respective radius parameters. In the end he decides to put four stars on the four corners of the image at very low magnitudes as a visual scale. Using all the information above, he creates the catalog of mock profiles he wants in a file named ‘cat.txt’ (short for catalog) using his favorite text editor and stores it in a directory named ‘simulationtest’ in his home directory. [The ‘cat’ command prints the contents of a file, short for concatenation. So please copy-paste the outputs of the command “‘cat cat.txt’†into ‘cat.txt’ when the editor opens in the steps above it, note that there are 6 lines]: $ mkdir ~/simulationtest $ cd ~/simulationtest $ pwd /home/rahman/simulationtest $ emacs cat.txt $ ls cat.txt $ cat cat.txt 0 0.0000 0.0000 1 5.000 4.765 0.0000 1.000 30.000 5.000 1 250.00 250.00 0 40.00 1.000 -25.00 0.400 3.4400 5.000 2 50.000 50.000 3 0.000 0.000 0.0000 0.000 9.0000 0.000 3 450.00 50.000 3 0.000 0.000 0.0000 0.000 9.2500 0.000 4 50.000 450.00 3 0.000 0.000 0.0000 0.000 9.5000 0.000 5 450.00 450.00 3 0.000 0.000 0.0000 0.000 9.7500 0.000 The zero-point magnitude for his observation was 18. Now he has all the necessary parameters and runs MakeProfiles with the following command: $ astmkprof --prepforconv --naxis1=500 --naxis2=500 \ --zeropoint=18.0 cat.txt MakeProfiles started on Sat Oct 6 16:26:56 953 - 6 profiles read from cat.txt in 0.000209 seconds ---- Row 5 complete, 5 left to go. ---- Row 3 complete, 4 left to go. ---- Row 2 complete, 3 left to go. ---- Row 4 complete, 2 left to go. ---- ./0_cat.fits created. ---- Row 0 complete, 1 left to go. ---- Row 1 complete, 0 left to go. - cat.fits created. in 0.024811 seconds MakeProfiles finished in: 0.236629 (seconds) $ls 0_cat.fits astmkprof.log cat.fits cat.txt The file ‘0.fits’ is the PSF Sufi had asked for and ‘cat.fits’ is the image containing the 5 objects. The PSF is now available to him as a separate file for the convolution step. While he was preparing the catalog, one of his students came up and was also following the steps. When he opened the image, the student was surprised to see that all the stars are only one pixel and not in the shape of the PSF as we see when we image the sky at night. So Sufi explained to him that the stars will take the shape of the PSF after convolution and this is how they would look if we didn’t have an atmosphere or an aperture when we took the image. The size of the image was also surprising for the student, instead of 500 by 500, it was 2630 by 2630 pixels. So Sufi had to explain why oversampling is very important for parts of the image where the flux change is significant over a pixel. Sufi then explained to him that after convolving we will re-sample the image to get our originally desired size. To convolve the image, Sufi ran the following command: $ astconvolve --kernel=0_cat.fits cat.fits Convolve started on Mon Apr 6 16:35:32 953 Convolving cat.fits (hdu: 0) with the kernel 0.fits (hdu: 0). using 8 CPU threads in the frequency domain. - Input and Kernel images padded. in 0.045576 seconds - Images converted to frequency domain. in 10.486712 seconds - Multiplied in the frequency domain. in 0.032780 seconds - Converted back to the spatial domain. in 5.342335 seconds - Padded parts removed. in 0.011880 seconds Convolve finished in: 15.972771 (seconds) $ls 0_cat.fits astmkprof.log cat_convolved.fits cat.fits cat.txt When convolution finished, Sufi opened the ‘cat_convolved.fits’ file and showed the effect of convolution to his student and explained to him how a PSF with a larger FWHM would make the points even wider. With the convolved image ready, they were ready to re-sample it to the original pixel scale Sufi had planned. Sufi explained the basic concepts of warping the image to his student and ran ImageWarp with the following command: $ astimgwarp cat_convolved.fits --scale=0.2 ImageWarp started on Mon Apr 6 16:51:59 953 Using 8 CPU threads. Input image: cat_convolved.fits matrix: 0.2000 0.0000 0.4000 0.0000 0.2000 0.4000 0.0000 0.0000 1.0000 ImageWarp finished in: 0.481421 (seconds) $ ls 0_cat.fits cat_convolved.fits cat.fits astmkprof.log cat_convolved_warped.fits cat.txt ‘cat_convolved_warped.fits’ now has the correct pixel scale. However, the image is still larger than what we had wanted, it is 526 ($500+13+13$) by 526 pixels. The student is slightly confused, so Sufi also resamples the PSF with ImageWarp and the same warping matrix and shows him that it is 27 ($2\times13+1$) by 27 pixels. Sufi goes on to explain how frequency space convolution will dim the edges and that is why he added the ‘--prepforconv’ option to MakeProfiles, see *note If convolving afterwards::. Now that convolution is done Sufi can remove those extra pixels using ImageCrop: $ astimgcrop cat_convolved_warped.fits --section=13:*-13,13:*-13 \ --zeroisnotblank ImageCrop started on Sat Oct 6 17:03:24 953 - Read metadata of 1 images. in 0.000560 seconds ---- cat_convolved_warped_crop.fits 1 1 ImageCrop finished in: 0.018917 (seconds) $ls 0_cat.fits astmkprof.log cat_convolved_warped.fits 0_warped.fits cat_convolved.fits cat.fits astimgcrop.log cat_convolved_warped_crop.fits cat.txt Finally, the ‘cat_convolved_warped.fits’ has the same dimensions as Sufi had asked for in the beginning. All this trouble was certainly worth it because now there is no dimming on the edges of the image and the profile centers are more accurately sampled. The final step to simulate a real observation would be to add noise to the image. Sufi set the zeropoint magnitude to the same value that he set when making the mock profiles and looking again at his observation log, he found that at that night the background flux near the nebula had a magnitude of 7. So using these values he ran MakeNoise: $ astmknoise --zeropoint=18 --background=7 --output=out.fits \ cat_convolved_warped_crop.fits MakeNoise started on Mon Apr 6 17:05:06 953 - Generator type: mt19937 - Generator seed: 1428318100 MakeNoise finished in: 0.033491 (seconds) $ls 0_cat.fits cat_convolved.fits cat.txt 0_warped.fits cat_convolved_warped_crop.fits out.fits astimgcrop.log cat_convolved_warped.fits astmkprof.log cat.fits The ‘out.fits’ file now has the noised image of the mock catalog Sufi had asked for. Seeing how the ‘--output’ option allows the user to specify the name of the output file, the student was confused and wanted to know why Sufi hadn’t used it before? Sufi then explained to him that for intermediate steps it is best to rely on the automatic output, see *note Automatic output::. Doing so will give all the intermediate files the same basic name structure, so in the end you can simply remove them all with the Shell’s capabilities. So Sufi decided to show this to the student by making a shell script from the commands he had used before. The command-line shell has the capability to read all the separate input commands from a file. This is very useful when you want to do the same thing multiple times, with only the names of the files or minor parameters changing between the different instances. Using the shell’s history (by pressing the up keyboard key) Sufi reviewed all the commands and then he retrieved the last 5 commands with the ‘$ history 5’ command. He selected all those lines he had input and put them in a text file named ‘mymock.sh’. Then he used some shell variables to set the two main constant parts of all the command to generalized variables. edge=13 base=cat rm out.fits astmkprof --prepforconv --naxis1=500 --naxis2=500 \ --zeropoint=18.0 "$base".txt astconvolve --kernel=0.fits "$base".fits astimgwarp "$base"_convolved.fits --scale=0.2 astimgcrop "$base"_convolved_warped.fits \ --section=$edge:*-$edge,$edge:*-$edge astmknoise --zeropoint=18 --background=7 --output=out.fits \ "$base"_convolved_warped_crop.fits rm 0*.fits cat*.fits *.log Sufi then explained to the eager student that you define a variable by giving it a name, followed by an ‘=’ sign and the value you want. Then you can reference that variable from anywhere in the script by calling its name with a ‘$’ prefix. So in the script whenever you see ‘$base’, the value we defined for it above is used. If you use advanced editors like GNU Emacs or even simpler ones like Gedit (part of the GNOME graphical user interface) the variables will become a different color which can really help in understanding the script. We have put all the ‘$base’ variables in double quotation marks (‘"’) so the variable name and the following text do not get mixed, the shell is going to ignore the ‘"’ after replacing the variable value. To make the script executable, Sufi ran the following command: $ chmod +x mymock.sh Then finally, Sufi ran the script, simply by calling its file name: $ ./mymock.sh After the script finished, the only file remaining is the ‘out.fits’ file that Sufi had wanted in the beginning. Sufi then explained to the student how he could run this script anywhere that he has a catalog if the script is in the same directory. The only thing the student had to modify in the script was the name of the catalog (the value of the ‘base’ variable in the start of the script) and the value to the ‘edge’ variable if he changed the PSF size. The student was also very happy to hear that he won’t need to make it executable again when he makes changes later, it will remain executable unless he explicitly changes the executable flag with ‘chmod’. The student was really excited, since now, through simple shell scripting, he could really speed up his work and run any command in any fashion he likes allowing him to be much more creative in his works. Until now he was using the graphical user interface which doesn’t have such a facility and doing repetitive things on it was really frustrating and some times he would make mistakes. So he left to go and try scripting on his own computer. Sufi could now get back to his own work and see if the simulated nebula which resembled the one in the Andromeda constellation could be detected or not. Although it was extremely faint(2), fortunately it passed his detection tests and he wrote it in the draft manuscript that would later become “Book of fixed starsâ€. He still had to check the other nebula he saw from Yemen and several other such objects, but they could wait until tomorrow (thanks to the shell script, he only has to define a new catalog). It was nearly sunset and they had to begin preparing for the night’s measurements on the ecliptic. ---------- Footnotes ---------- (1) Abd al-rahman Sufi (903 – 986 A.D.), also known in Latin as Azophi was an Iranian astronomer. His manuscript “Book of fixed stars†contains the first recorded observations of the Andromeda galaxy, the Large Magellanic Cloud and seven other non-stellar or ‘nebulous’ objects. (2) The brightness of a diffuse object is added over all its pixels to give its final magnitude, see *note Flux Brightness and magnitude::. So although the magnitude 3.44 (of the mock nebula) is orders of magnitude brighter than 6 (of the stars), the central galaxy is much fainter. Put another way, the brightness is distributed over a large area in the case of a nebula.  File: gnuastro.info, Node: Installation, Next: Common program behavior, Prev: Tutorials, Up: Top 3 Installation ************** To successfully install and thus use Gnuastro, first please make sure you have the dependencies installed (see *note Dependencies::). Only the first group are required when you are building Gnuastro using a tarball (see *note Release tarball::), they are very basic and low-level tools used in most astronomical software, so you might already have them installed, if not they are very easy to install as described for each. *note Downloading the source:: discusses the two methods you can obtain the source code: as a tarball (a significant snapshot in Gnuastro’s history), or the full history. The building and installation of Gnuastro is heavily customizable, to learn more about them, see *note Build and install::. This section is essentially a thorough explanation of the steps in *note Quick start::. It discusses ways you can influence the building and installation. If you encounter any problems in the installation process, it is probably already explained in *note Known issues::. In *note Other useful software:: the installation and usage of some other free software that are not directly required by Gnuastro but might be useful in conjunction with it is discussed. * Menu: * Dependencies:: Necessary packages for Gnuastro. * Downloading the source:: Ways to download the source code. * Build and install:: Configure, build and install Gnuastro.  File: gnuastro.info, Node: Dependencies, Next: Downloading the source, Prev: Installation, Up: Installation 3.1 Dependencies ================ The dependencies needed to build and install Gnuastro are defined by the features you want and how you would like to obtain the source code (see *note Downloading the source::). A minimal set of dependencies are mandatory, if they are not present you cannot get passed the configuration step. Such mandatory dependencies are therefore very basic (low-level) tools which are easy to obtain, build and install, see *note Mandatory dependencies:: for a full discussion. If you have the packages of *note Optional dependencies::, Gnuastro will have additional functionality (for example converting FITS images to JPEG or PDF). If you are installing from a tarball as explained in *note Quick start::, you can stop reading after this section. However, if you decided to use the version controlled source instead of the tarball (see *note Version controlled source::), an additional bootstrapping step is required before configuration and its dependencies are explained in *note Bootstrapping dependencies::. * Menu: * Mandatory dependencies:: Gnuastro will not install without these. * Optional dependencies:: Adding more functionality. * Bootstrapping dependencies:: If you have the version controlled source.  File: gnuastro.info, Node: Mandatory dependencies, Next: Optional dependencies, Prev: Dependencies, Up: Dependencies 3.1.1 Mandatory dependencies ---------------------------- The mandatory Gnuastro dependencies are very basic and low-level tools. They all follow the same basic GNU based build system (like that shown in *note Quick start::), so even if you don’t have them, installing them should be pretty straightforward. In this section we explain each program and any specific note that might be necessary in the installation. The most basic choice is to build the packages from source yourself, instead of relying on your distribution’s package management system. While the latter choice is indeed possible, we recommend that you build these dependencies yourself as discussed below. We will send out notifications in the ‘info-gnuastro’ mailing list, see *note Announcements:: when we find out that these requirements are updated. 1. For each package, Gnuastro might preform better (or require) certain configuration options that your distribution’s package managers didn’t add for you. If present, these configuration options are explained during the installation of each in the sections below. When the proper configuration has not been set, the programs should complain and inform you. 2. Your distribution’s pre-built package might not be the most recent release. 3. For the libraries, they might separate the binary file from the header files, see *note Known issues::. 4. Like any other tool, the science you derive from Gnuastro’s tools highly depend on these lower level dependencies, so generally it is much better to have a close connection with them. By reading their manuals, installing them and staying up to date with changes/bugs in them, your scientific results and understanding will also correspondingly improve. * Menu: * GNU Scientific Library:: Installing GSL. * CFITSIO:: C interface to the FITS standard. * WCSLIB:: C interface to the WCS standard of FITS.  File: gnuastro.info, Node: GNU Scientific Library, Next: CFITSIO, Prev: Mandatory dependencies, Up: Mandatory dependencies 3.1.1.1 GNU Scientific library .............................. The GNU Scientific Library (http://www.gnu.org/software/gsl/), or GSL, is a large collection of functions that are very useful in scientific applications, for example integration, random number generation, and Fast Fourier Transform among many others. To install GSL from source, you can run the following commands after you have downloaded ‘gsl-latest.tar.gz’ (ftp://ftp.gnu.org/gnu/gsl/gsl-latest.tar.gz): $ tar xf gsl-latest.tar.gz $ cd gsl-X.X # Replace X.X with version number $ ./configure $ make $ make check $ sudo make install  File: gnuastro.info, Node: CFITSIO, Next: WCSLIB, Prev: GNU Scientific Library, Up: Mandatory dependencies 3.1.1.2 CFITSIO ............... CFITSIO (http://heasarc.gsfc.nasa.gov/fitsio/) is the closest you can get to the pixels in a FITS image while remaining faithful to the FITS standard (http://fits.gsfc.nasa.gov/fits_standard.html). It is written by William Pence, the principal author of the FITS standard(1), and is regularly updated. Setting the definitions for all other software packages using FITS images. Some GNU/Linux distributions have CFITSIO in their package managers, if it is available and updated, you can use it. One problem that might occur is that CFITSIO might not be configured with the ‘--enable-reentrant’ option by the distribution. This option allows CFITSIO to open a file in multiple threads, it can thus provide great speed improvements. If CFITSIO was not configured with this option, any program which needs this capability will warn you and abort when you ask for multiple threads (see *note Threads in Gnuastro::). To install CFITSIO from source, we strongly recommend that you have a look through Chapter 2 (Creating the CFITSIO library) of the CFITSIO manual and understand the options you can pass to ‘$ ./configure’ (they aren’t too much). This is a very basic package for most astronomical software and it is best that you configure it nicely with your system. Once you download the source and unpack it, the following configure script should be enough for most purposes. Don’t forget to read chapter two of the manual though, for example the second option is only for 64bit systems. The manual also explains how to check if it has been installed correctly. CFITSIO comes with two executables called fpack and funpack. From their manual: they “are standalone programs for compressing and uncompressing images and tables that are stored in the FITS (Flexible Image Transport System) data format. They are analogous to the gzip and gunzip compression programs except that they are optimized for the types of astronomical images that are often stored in FITS formatâ€. The instruction below explain how to compile and install them on your system along with CFITSIO. They are not essential for Gnuastro, since they are just wrappers for functions within CFITSIO, but they can come in handy. The ‘make utils’ command is only available for versions above 3.39, it will build these executables along with several other test executables which are deleted before the installation (otherwise they will also be installed). The CFITSIO installation from source process is given below. Let’s assume you have downloaded ‘cfitsio_latest.tar.gz’ (http://heasarc.gsfc.nasa.gov/FTP/software/fitsio/c/cfitsio_latest.tar.gz) and are in the same directory: $ tar xf cfitsio_latest.tar.gz $ cd cfitsio $ ./configure --prefix=/usr/local --enable-sse2 --enable-reentrant $ make $ make utils $ ./testprog > testprog.lis $ diff testprog.lis testprog.out # Should have no output $ cmp testprog.fit testprog.std # Should have no output $ rm cookbook fitscopy imcopy smem speed testprog $ sudo make install ---------- Footnotes ---------- (1) Pence, W.D. et al. Definition of the Flexible Image Transport System (FITS), version 3.0. (2010) Astronomy and Astrophysics, Volume 524, id.A42, 40 pp.  File: gnuastro.info, Node: WCSLIB, Prev: CFITSIO, Up: Mandatory dependencies 3.1.1.3 WCSLIB .............. WCSLIB (http://www.atnf.csiro.au/people/mcalabre/WCS/) is written and maintained by one of the authors of the World Coordinate System (WCS) definition in the FITS standard (http://fits.gsfc.nasa.gov/fits_standard.html)(1), Mark Calabretta. It might be already built and ready in your distribution’s package management system. However, here the installation from source is explained, for the advantages please see *note Mandatory dependencies::. To install WCSLIB you will need to have CFITSIO already installed, see *note CFITSIO::. WCSLIB also has plotting capabilities which use PGPLOT (a plotting library for C). If you wan to use those capabilities in WCSLIB, *note PGPLOT:: provides the PGPLOT installation instructions. However PGPLOT is old(2), so its installation is not easy, there are also many great modern WCS plotting tools (mostly in written in Python). Hence, if you will not be using those plotting functions in WCSLIB, you can configure it with the ‘--without-pgplot’ option as shown below. Let’s assume you have downloaded ‘wcslib.tar.bz2’ (ftp://ftp.atnf.csiro.au/pub/software/wcslib/wcslib.tar.bz2) and are in the same directory: $ tar xf wcslib.tar.bz2 $ cd wcslib-X.X # Replace X.X with version number $ ./configure --without-pgplot LIBS="-pthread -lm" $ make $ make check $ sudo make install ---------- Footnotes ---------- (1) Greisen E.W., Calabretta M.R. (2002) Representation of world coordinates in FITS. Astronomy and Astrophysics, 395, 1061-1075. (2) As of early June 2016, its most recent version was uploaded in February 2001.  File: gnuastro.info, Node: Optional dependencies, Next: Bootstrapping dependencies, Prev: Mandatory dependencies, Up: Dependencies 3.1.2 Optional dependencies --------------------------- The libraries listed here are only used for very specific applications, therefore if you don’t want these operations, Gnuastro will be built and installed without them and you don’t have to have the dependencies. If the ‘./configure’ script can’t find these requirements, it will warn you in the end that they are not present and notify you of the operation(s) you can’t do due to not having them. If the output you request from a program requires a missing library, that program is going to warn you and abort. In the case of executables like GPL GhostScript, if you install them at a later time, the program will run. This is because if required libraries are not present at build time, the executables cannot be built, but an executable is called by the built program at run time so if it becomes available, it will be used. If you do install an optional library later, you will have to rebuild Gnuastro and reinstall it for it to take effect. libgit2 Git is one of the most common version control systems (see *note Version controlled source::). When ‘libgit2’ is present, all Gnuastro’s outputs will contain the version number of the working directory’s repository for future reproducibility. See the ‘COMMIT’ keyword header in *note Output headers:: for a discussion. libjpeg libjpeg is only used by ConvertType to read from and write to JPEG images. libjpeg (http://www.ijg.org/) is a very basic library that provides tools to read and write JPEG images, most of the GNU/Linux graphic programs and libraries use it. Therefore you most probably already have it installed. libjpeg-turbo (http://libjpeg-turbo.virtualgl.org/) is an alternative to libjpeg. It uses SIMD instructions for ARM based systems that significantly decreases the processing time of JPEG compression and decompression algorithms. GPL Ghostscript GPL Ghostscript’s executable (‘gs’) is called used by ConvertType to compile a PDF file from a source PostScript file, see *note ConvertType::. Therefore its headers (and libraries) are not needed. With a very high probability you already have it in your GNU/Linux distribution. Unfortunately it does not follow the standard GNU build style so installing it is very hard. It is best to rely on your distribution’s package managers for this.  File: gnuastro.info, Node: Bootstrapping dependencies, Prev: Optional dependencies, Up: Dependencies 3.1.3 Bootstrapping dependencies -------------------------------- Bootstrapping is only necessary if you have decided to obtain the full version controlled history of Gnuastro, see *note Version controlled source:: and *note Bootstrapping::. Using the version controlled source enables you to always be up to date with the most recent development work of Gnuastro (bug fixes, new functionalities, improved algorithms and etc). If you have downloaded a tarball (see *note Downloading the source::), then you can ignore this subsection. To successfully run the bootstrapping process, there are some additional dependencies to those discussed in the previous subsections. These are low level tools that are used by a large collection of Unix-like operating systems programs, therefore they are most probably already available in your system. If they are not already installed, you should be able to easily find them in any GNU/Linux distribution package management system (‘apt-get’, ‘yum’, ‘pacman’ and etc). The short names in parenthesis in ‘typewriter’ font after the package name can be used to search for them in your package manager. For the GNU Portability Library, GNU Autoconf Archive and TeX Live, it is recommended to use the instructions here, not your operating system’s package manager. GNU Portability Library (Gnulib) To ensure portability for a wider range of operating systems (those that don’t include GNU C library, namely glibc), Gnuastro depends on the GNU portability library, or Gnulib. Gnulib keeps a copy of all the functions in glibc, implemented (as much as possible) to be portable to other operating systems. The ‘bootstrap’ script can automatically clone Gnulib (as a ‘gnulib/’ directory inside Gnuastro), however, as described in *note Bootstrapping:: this is not recommended. The recommended way to bootstrap Gnuastro is to first clone Gnulib and the Autoconf archives (see below) into a local directory outside of Gnuastro. Let’s call it ‘DEVDIR’(1) (which you can set to any directory). Currently in Gnuastro, both Gnulib and Autoconf archives have to be cloned in the same top directory(2) like the case here(3): $ DEVDIR=/home/yourname/Development $ cd $DEVDIR $ git clone git://git.sv.gnu.org/gnulib.git $ git clone git://git.sv.gnu.org/autoconf-archive.git You now have the full version controlled source of these two repositories in separate directories. Both these packages are regularly updated, so every once in a while, you can run ‘$ git pull’ within them to get any possible updates. GNU Automake (‘automake’) GNU Automake will build the ‘Makefile.in’ files in each sub-directory using the (hand-written) ‘Makefile.am’ files. The ‘Makefile.in’s are subsequently used to generate the ‘Makefile’s when the user runs ‘./configure’ before building. GNU Autoconf (‘autoconf’) GNU Autoconf will build the ‘configure’ script using the configurations we have defined (hand-written) in ‘configure.ac’. GNU Autoconf Archive These are a large collection of tests that can be called to run at ‘./configure’ time. See the explanation under GNU Portability Library above for instructions on obtaining it and keeping it up to date. GNU Libtool (‘libtool’) GNU Libtool is in charge of building all the libraries in Gnuastro. The libraries contain functions that are used by more than one program and are installed for use in other programs. They are thus put in a separate directory (‘lib/’). GNU help2man (‘help2man’) GNU help2man is used to convert the output of the ‘--help’ option (*note --help::) to the traditional Man page (*note Man pages::). LaTeX and some TeX packages Some of the figures in this book are built by LaTeX (using the PGF/TikZ package). The LaTeX source for those figures is version controlled for easy maintenance not the actual figures. So the ‘./boostrap’ script will run LaTeX to build the figures. The best way to install LaTeX and all the necessary packages is through TeX live (https://www.tug.org/texlive/) which is a package manager for TeX related tools that is independent of any operating system. It is thus preferred to the TeX Live versions distributed by your operating system. To install TeX Live, go to the webpage and download the appropriate installer by following the “download†link. Note that by default the full package repository will be downloaded and installed (around 4 Giga Bytes) which can take _very_ long to download and to update later. However, most packages are not needed by everyone, it is easier, faster and better to install only the “Basic scheme†(consisting of only the most basic TeX and LaTeX packages, which is less than 200 Mega bytes)(4). After the installation be sure to set the environment variables as suggested in the end of the outputs. Any time you confront (need) a package you don’t have, simply install it with a command like below (similar to how you install software from your operating system’s package manager)(5). To install all the necessary TeX packages for a successful Gnuastro bootstrap, run this command: $ su # tlmgr install epsf jknapltx caption biblatex biber iftex \ etoolbox logreq xstring xkeyval pgf ms \ xcolor pgfplots times rsfs pstools epspdf ImageMagick (‘imagemagick’) ImageMagick is a wonderful and robust program for image manipulation on the command-line. ‘bootsrap’ uses it to convert the book images into the formats necessary for the various book formats. ---------- Footnotes ---------- (1) If you are not a developer in Gnulib or Autoconf archives, ‘DEVDIR’ can be a directory that you don’t backup. In this way the large number of files in these projects won’t slow down your backup process or take bandwidth (if you backup to a remote server). (2) If you already have the Autoconf archives in a separate directory, or can’t clone it in the same directory as Gnulib, or you have it with another directory name (not ‘autoconf-archive/’), you can follow this short step. Set ‘AUTOCONFARCHIVES’ to your desired address. Then define a symbolic link in ‘DEVDIR’ with the following command so Gnuastro’s bootstrap script can find it: ‘$ ln -s $AUTOCONFARCHIVES $DEVDIR/autoconf-archive’. (3) If your internet connection is active, but Git complains about the network, it might be due to your network setup not recognizing the git protocol. In that case use the following URL for the HTTP protocol instead (for Autoconf archives, replace the name): ‘http://git.sv.gnu.org/r/gnulib.git’ (4) You can also download the DVD iso file at a later time to keep as a backup for when you don’t have internet connection if you need a package. (5) After running TeX, or LaTeX, you might get a warning complaining about a ‘missingfile’. Run ‘‘tlmgr info missingfile’’ to see the package(s) containing that file which you can install.  File: gnuastro.info, Node: Downloading the source, Next: Build and install, Prev: Dependencies, Up: Installation 3.2 Downloading the source ========================== Gnuastro’s source code can be downloaded in two ways. As a tarball, ready to be configured and installed on your system (as described in *note Quick start::), see *note Release tarball::. If you want official releases of stable versions this is the best, easiest and most common option. Alternatively, you can clone the version controlled history of Gnuastro, run one extra bootstrapping step and then follow the same steps as the tarball. This will give you access to all the most recent work that will be included in the next release along with the full project history. The process is thoroughly introduced in *note Version controlled source::. * Menu: * Release tarball:: Download a stable official release. * Version controlled source:: Get and use the version controlled source.  File: gnuastro.info, Node: Release tarball, Next: Version controlled source, Prev: Downloading the source, Up: Downloading the source 3.2.1 Release tarball --------------------- A release tarball (commonly compressed) is the most common way of obtaining free and open source software. A tarball is a snapshot of one particular moment in the Gnuastro development history along with all the necessary files to configure, build, and install Gnuastro easily (see *note Quick start::). It is very straightforward and needs the least set of dependencies (see *note Mandatory dependencies::). Gnuastro has tarballs for official stable releases and pre-releases for testing. See *note Version numbering:: for more on the two types of releases and the formats of the version numbers. The URLs for each type of release are given below. Official stable releases (): This URL hosts the official stable releases of Gnuastro. Always use the most recent version (see *note Version numbering::). By clicking on the “Last modified†title of the second column, the files will be sorted by their date which you can also use to find the latest version. It is recommended to use a mirror to download these tarballs, please visit and see below. Pre-release tar-balls (): This URL contains unofficial pre-release versions of Gnuastro. The pre-release versions of Gnuastro here are for enthusiasts to try out before an official release. If there are problems, or bugs then the testers will inform the developers to fix before the next official release. See *note Version numbering:: to understand how the version numbers here are formatted. If you want to remain even more up-to-date with the developing activities, please clone the version controlled source as described in *note Version controlled source::. Gnuastro’s official tarball is released with two formats: Gzip (with suffix ‘.tar.gz’) and Lzip (with suffix ‘.tar.lz’). The former is a very well-known and widely used compression program created by GNU and available in most systems. The latter provides a better compression ratio and more robust archival capacity. For example Gnuastro 0.2’s tarball was 2.8MB and 4.2MB with Lzip and Gzip respectively. From the Lzip webpage (http://www.nongnu.org/lzip/lzip.html): “Lzip is a lossless data compressor with a user interface similar to the one of gzip or bzip2. Lzip can compress about as fast as gzip (‘lzip -0’), or compress most files more than bzip2 (‘lzip -9’). Decompression speed is intermediate between gzip and bzip2. Lzip is better than gzip and bzip2 from a data recovery perspective.†However, Lzip is currently not too common, so it might not be pre-installed in your operating system. Installing it from your operating system’s package manager or from source is very easy. The GNU FTP server is mirrored (has backups) in various locations on the globe (). You can use the closest mirror to your location for a more faster download. Note that only some mirrors keep track of the pre-release (alpha) tarballs. Also note that if you want to download immediately after and announcement (see *note Announcements::), the mirrors might need some time to synchronize with the main GNU FTP server.  File: gnuastro.info, Node: Version controlled source, Prev: Release tarball, Up: Downloading the source 3.2.2 Version controlled source ------------------------------- The publicly distributed Gnuastro tar-ball (for example ‘gnuastro-X.X.tar.gz’) does not contain the revision history, it is only a snapshot of the source code at one significant instant of Gnuastro’s history (specified by the version number, see *note Version numbering::), ready to be configured and built. To be able to develop successfully, the revision history of the code can be very useful to track when something was added or changed, also some updates that are not yet officially released might be in it. We use Git for the version control of Gnuastro. For those who are not familiar with it, we recommend the Pro Git(1) book. The whole book is publicly available for online reading and downloading and does a wonderful job at explaining the concepts and best practices. Let’s assume you want to keep Gnuastro in the ‘TOPGNUASTRO’ directory (can be any directory, change the value below). The full version controlled history of Gnuastro can be cloned in ‘TOPGNUASTRO/gnuastro’ by running the following commands(2): $ TOPGNUASTRO=/home/yourname/Research/projects/ $ cd $TOPGNUASTRO $ git clone git://git.sv.gnu.org/gnuastro.git The ‘$TOPGNUASTRO/gnuastro’ directory will contain hand-written (version controlled) source code for Gnuastro’s programs, libraries, this book and the tests. All are divided into sub-directories with standard and very descriptive names. The version controlled files in the top cloned directory are either mainly in capital letters (for example ‘THANKS’ and ‘README’) or mainly written in small-caps (for example ‘configure.ac’ and ‘Makefile.am’). The former are non-programming, standard writing for human readers containing high-level information about the whole package. The latter are instructions to customize the GNU build system for Gnuastro. The cloned Gnuastro source cannot immediately be configured, compiled, or installed since it only contains hand-written files, not automatically generated or imported files which do all the hard work of the build process. See *note Bootstrapping:: for the process of generating and importing those files (it is very easy!). Once you have bootstrapped Gnuastro, you can run the standard procedures (in *note Quick start::). Very soon after you have cloned it, Gnuastro’s main ‘master’ branch will be updated on the main repository (since the developers are actively working on Gnuastro), for the best practices in keeping your local history in sync with the main repository see *note Synchronizing::. * Menu: * Bootstrapping:: Adding all the automaticly generated files. * Synchronizing:: Keep your local clone up to date. ---------- Footnotes ---------- (1) (2) If your internet connection is active, but Git complains about the network, it might be due to your network setup not recognizing the Git protocol. In that case use the following URL which uses the HTTP protocol instead: ‘http://git.sv.gnu.org/r/gnuastro.git’  File: gnuastro.info, Node: Bootstrapping, Next: Synchronizing, Prev: Version controlled source, Up: Version controlled source 3.2.2.1 Bootstrapping ..................... The version controlled source code lacks the source files that we have not written or are automatically built. These automatically generated files are included in the distributed tar ball for each distribution (for example ‘gnuastro-X.X.tar.gz’, see *note Version numbering::) and make it easy to immediately configure, build, and install Gnuastro. However from the perspective of version control, they are just bloatware and sources of confusion (since they are not changed by Gnuastro developers). The process of automatically building and importing necessary files into the cloned directory is known as _bootstrapping_. All the instructions for an automatic bootstrapping are available in ‘bootstrap’ and configured using ‘bootstrap.conf’. ‘bootstrap’ is the only file not written by Gnuastro developers but is under version control to enable simple bootstrapping immediately after cloning. It is maintained by the GNU Portability Library (Gnulib) and this file is an identical copy, so do not make any changes in this file since it will be replaced when Gnulib releases an update. Make all your changes in ‘bootstrap.conf’. The bootstrapping process has its own separate set of dependencies, the full list is given in *note Bootstrapping dependencies::. They are generally very low-level and used by a very large set of commonly used programs, so they are probably already installed on your system. The simplest way to bootstrap Gnuastro is to simply run the bootstrap script within your cloned Gnuastro directory as shown below. However, please read the next paragraph before doing so (see *note Version controlled source:: for ‘TOPGNUASTRO’). $ cd TOPGNUASTRO/gnuastro $ ./bootstrap # Requires internet connection Without any options, ‘bootstrap’ will clone Gnulib within your cloned Gnuastro directory (‘TOPGNUASTRO/gnuastro/gnulib’) and download the necessary Autoconf archives macros. So if you run bootstrap like this, you will need an internet connection every time you decide to bootstrap. Also, Gnulib is a large package and cloning it can be slow. It will also keep the full Gnulib repository within your Gnuastro repository, so if another one of your projects also needs Gnulib, and you insist on running bootstrap like this, you will have two copies. In case you regularly backup your important files, Gnulib will also slow down the backup process. Therefore while the simple invocation above can be used with no problem, it is not recommended, see the next paragraph. The recommended way to get these two packages is thoroughly discussed in *note Bootstrapping dependencies:: (in short: clone them in the separate ‘DEVDIR/’ directory). The following commands will take you into the cloned Gnuastro directory and run the ‘bootstrap’ script, while telling it to copy some files (instead of making symbolic links, with the ‘--copy’ option, this is not mandatory(1)) and where to look for Gnulib (with the ‘--gnulib-srcdir’ option). $ cd $TOPGNUASTRO/gnuastro $ ./bootstrap --copy --gnulib-srcdir=$DEVDIR/gnulib Since Gnulib and Autoconf archives are now available in your local directories, you don’t need an internet connection every time you decide to remove all untracked files and redo the bootstrap (see box below). You can also use the same command on any other project that uses Gnulib. All the necessary GNU C library functions, Autoconf macros and Automake inputs are now available along with the book figures. The standard GNU build system (*note Quick start::) will do the rest of the job. *Undoing the bootstrap:* During the development, it might happen that you want to remove all the automatically generated and imported files. In other words, you might want to reverse the bootstrap process. Fortunately Git has a good program for this job: ‘git clean’. Run the following command and every file that is not version controlled will be removed. git clean -fxd It is best to commit any recent change before running this command. You might have created new files since the last commit and if they haven’t been committed, they will all be gone forever (using ‘rm’). To get a list of the non-version controlled files instead of deleting them, add the ‘n’ option to ‘git clean’, so it becomes ‘-fxdn’. Besides the ‘bootstrap’ and ‘bootstrap.conf’, the ‘bootstrapped/’ directory and ‘README-hacking’ file are also related to the bootstrapping process. The former hosts all the imported (bootstrapped) directories. Thus, in the version controlled source, it only contains a ‘REAME’ file, but in the distributed tar-ball it also contains sub-directories filled with all bootstrapped files. ‘README-hacking’ contains a summary of the bootstrapping process discussed in this section. It is a necessary reference when you haven’t built this book yet. It is thus not distributed in the Gnuastro tarball. ---------- Footnotes ---------- (1) The ‘--copy’ option is recommended because some backup systems might do strange things with symbolic links.  File: gnuastro.info, Node: Synchronizing, Prev: Bootstrapping, Up: Version controlled source 3.2.2.2 Synchronizing ..................... The bootstrapping script (see *note Bootstrapping::) is not regularly needed: you mainly need it after you have cloned Gnuastro (once) and whenever you want to re-import the files from Gnulib, or Autoconf archives(1) (not too common). However, Gnuastro developers are constantly working on Gnuastro and are pushing their changes to the official repository. Therefore, your local Gnuastro clone will soon be out-dated. Gnuastro has two mailing lists dedicated to its developing activities (see *note Developing mailing lists::). Subscribing to them can help you decide when to synchronize with the official repository. To pull all the most recent work in Gnuastro, run the following command from the top Gnuastro directory: $ git pull && autoconf -f GNU Autoconf is part of the GNU build system and will update the ‘./configure’ script based on the hand-written configurations (in ‘configure.ac’, which is version controlled in Gnuastro). The pulled changes might contain changes in the build system configurations. However, The most important reason for running this command is to generate a version number for your Gnuastro snapshot. This generated version number will include the commit information if you are building Gnuastro from any point in Gnuastro’s history (see *note Version numbering::). Since the version number is included in nearly all outputs of the programs, this can help you later exactly reproduce an old result by checking out the exact point in Gnuastro’s history that produced those results. Therefore, be sure to run ‘‘autoconf -f’’ after every synchronization. You can also run them separately: $ git pull $ autoconf -f If you would like to see what has changed since you last synchronized your local clone, you can take the following steps instead of the simple command above (don’t type anything after ‘#’): $ git checkout master # Confirm if you are on master. $ git fetch origin # Fetch all new commits from server. $ git log master..origin/master # See all the new commit messages. $ git merge origin/master # Update your master branch. $ autoconf -f # Update ./configure. By default ‘git log’ prints the most recent commit first, add the ‘--reverse’ option to see the changes chronologically. To see exactly what has been changed in the source code along with the commit message, add a ‘-p’ option to the ‘git log’. If you intend make changes in the code, have a look at *note Developing:: to get started easily. Be sure to commit your changes in a separate branch (keep your ‘master’ branch to follow the official repository) and re-run ‘autoconf -f’ after the commit. If you intend to send your changes to us (see *note Contributing to Gnuastro::) for the benefit of the whole community. If you send your work to us, you can safely use your commit since it will be ultimately recorded in Gnuastro’s official history. If not, please upload your separate branch to a public hosting service (for example GitLab, see *note Forking tutorial::) and link to it in your report, or run ‘make distcheck’ and upload the output ‘gnuastro-X.X.X.XXXX.tar.gz’ to a publicly accessible webpage so your results can be considered scientific (reproducible). ---------- Footnotes ---------- (1) is defined for you to check if significant (for Gnuastro) updates are made in these repositories, since the last time you pulled from them.  File: gnuastro.info, Node: Build and install, Prev: Downloading the source, Up: Installation 3.3 Build and install ===================== This section is basically a longer explanation to the sequence of commands given in *note Quick start::. If you didn’t have any problems during the *note Quick start:: steps, you want to have all the programs of Gnuastro installed in your system, you don’t want to change the executable names during or after installation, you have root access to install the programs in the default system wide directory, the Letter paper size of the print book is fine for you or as a summary you don’t feel like going into the details when everything is working, you can safely skip this section. If you have any of the above problems or you want to understand the details for a better control over your build and install, read along. The dependencies which you will need prior to configuring, building and installing Gnuastro are explained in *note Dependencies::. The first three steps in *note Quick start:: need no extra explanation, so we will skip them and start with an explanation of Gnuastro specific configuration options and a discussion on the installation directory in *note Configuring::, followed by some smaller subsections: *note Tests::, *note A4 print book::, and *note Known issues:: which explains the solutions to known problems you might encounter in the installation steps and ways you can solve them. * Menu: * Configuring:: Configure Gnuastro * Tests:: Run tests to see if it is working. * A4 print book:: Customize the print book. * Known issues:: Issues you might encounter.  File: gnuastro.info, Node: Configuring, Next: Tests, Prev: Build and install, Up: Build and install 3.3.1 Configuring ----------------- The ‘$ ./configure’ step is the most important step in the build and install process. All the required packages, libraries, headers and environment variables are checked in this step. The behaviors of make and make install can also be set through command line options to this command. The configure script accepts various arguments and options which enable the final user to highly customize whatever she is building. The options to configure are generally very similar to normal program options explained in *note Arguments and options::. Similar to all GNU programs, you can get a full list of the options along with a short explanation by running $ ./configure --help A complete explanation is also included in the ‘INSTALL’ file. Note that this file was written by the authors of GNU Autoconf (which builds the ‘configure’ script), therefore it is common for all programs which use the ‘$ ./configure’ script for building and installing, not just Gnuastro. Here we only discuss cases where you don’t have super-user access to the system and if you want to change the executable names. But before that, a review of the options to configure that are particular to Gnuastro are discussed. * Menu: * Gnuastro configure options:: Configure options particular to Gnuastro. * Installation directory:: Specify the directory to install. * Executable names:: Changing executable names. * Configure and build in RAM:: For minimal use of HDD or SSD, and clean source.  File: gnuastro.info, Node: Gnuastro configure options, Next: Installation directory, Prev: Configuring, Up: Configuring 3.3.1.1 Gnuastro configure options .................................. Most of the options to configure (which are to do with building) are similar for every program which uses this script. Here the options that are particular to Gnuastro are discussed. The next topics explain the usage of other configure options which can be applied to any program using the GNU build system (through the configure script). ‘--enable-progname’ Only build and install ‘progname’ along with any other program that is enabled in this fashion. ‘progname’ is the name of the executable without the ‘ast’, for example ‘imgcrop’ for ImageCrop (with the executable name of ‘astimgcrop’). If this option is called for any of the programs in Gnuastro, any program which is not explicitly enabled will not be built or installed. ‘--disable-progname’ ‘--enable-progname=no’ Do not build or install the program named ‘progname’. This is very similar to the ‘--enable-progname’, but will build and install all the other programs except this one. ‘--enable-gnulibcheck’ Enable checks on the GNU Portability Library (Gnulib). Gnulib is used by Gnuastro to enable users of non-GNU based operating systems (that don’t use GNU C library or glibc) to compile and use the advanced features that this library provides. We make extensive use of such functions. If you give this option to ‘$ ./configure’, when you run ‘$ make check’, first the functions in Gnulib will be tested, then the Gnuastro executables. If your operating system does not support glibc or has an older version of it and you have problems in the build process (‘$ make’), you can give this flag to configure to see if the problem is caused by Gnulib not supporting your operating system or Gnuastro, see *note Known issues::. ‘--disable-guide-message’ ‘--enable-guide-message=no’ Do not print a guiding message during the GNU Build process of *note Quick start::. By default, after each step, a message is printed guiding the user what the next command should be. Therefore, after ‘./configure’, it will suggest running ‘make’. After ‘make’, it will suggest running ‘make check’ and so on. If Gnuastro is configured with this option, for example $ ./configure --disable-guide-message Then these messages will not be printed after any step (like most programs). For people who are not yet fully accustomed to this build system, these guidelines can be very useful and encouraging. However, if you find those messages annoying, use this option. *Note:* If some programs are enabled and some are disabled, it is equivalent to simply enabling those that were enabled. Listing the disabled programs is redundant. Note that the tests of some programs might require other programs to have been installed and tested. For example MakeProfiles is the first program to be tested when you run ‘$ make check’, it provides the inputs to all the other tests. So if you don’t install MakeProfiles, then the tests for all the other programs will be skipped or fail. To avoid this, in one run, you can install all the packages and run the tests but not install. If everything is working correctly, you can run configure again with only the packages you want but not run the tests and directly install after building.  File: gnuastro.info, Node: Installation directory, Next: Executable names, Prev: Gnuastro configure options, Up: Configuring 3.3.1.2 Installation directory .............................. One of the most commonly used options to configure is the directory that will host all the files which require installing (for example the actual executable files for the program and/or the documentation and configuration files). This is done through the ‘--prefix’ option. To demonstrate its applicability, let’s assume you don’t have administrator or root access but you want to be able to access the installed files from anywhere while you are logged in (one of the most common uses of ‘--prefix’). The most basic way to run an executable is to explicitly type the full file name (including all the directory information) and run it. One example is running the configuration script with the ‘$ ./configure’ command (see *note Quick start::). By giving a specific directory (the current directory or ‘./’), we are explicitly telling the shell to look in the current directory for an executable file named ‘‘configure’’. Directly specifying the directory is thus useful for simple shell scripts in the current (or nearby) directories. However, when the program (an executable) is to be used a lot, specifying all those directories will become a significant burden. For example, the ‘ls’ executable lists the contents in a given directory and it is (usually) installed in the ‘/usr/bin/’ directory by the operating system maintainers. So each time you you want to use it you would have to run the following command (which is very inconvenient, both in typing and in remembering the various directories). $ /usr/bin/ls To address this problem, we have the ‘PATH’ environment variable. To understand it better, we will start with a short introduction to the shell variables. Shell variable values are basically treated as strings of characters. You can define a variable and a value for it by running $ myvariable=a_test_value You can see the value it represents by running $ echo $myvariable If a variable has no value, the last command will only print an empty line. A variable defined like this will be known as long as this shell or terminal is running. Other terminals will have no idea it existed. The main advantage of shell variables is that if they are exported(1), subsequent programs that are run within that shell can access their value. So by giving them different values, you can change the “environment†of a program which uses their values. The shell variables which are accessed by programs are therefore known as “environment variablesâ€(2). You can see the full list of the environment variables that your shell currently recognizes by running: $ printenv ‘HOME’ is one commonly used environment variable, it is any user’s (the one that is logged in) top directory. It is used so often that the shell has a special expansion (alternative) for it: ‘‘~’’. Whenever you see file names starting with the tilde sign, it actually represents the value to the ‘HOME’ environment variable, so ‘~/doc’ is the same as ‘$HOME/doc’. Another one of the most commonly used environment variables is ‘PATH’, it is a list of directories to search for executable names. Its value is a list of directories (separated by a colon, or ‘<:>’). When the address of the executable is not explicitly given (like ‘./configure’ above), the system will look for the executable in the directories specified by ‘PATH’. If you have a computer nearby, try running the following command to see which directories your system will look into when it is searching for executable (binary) files, one example is printed here (notice how ‘/usr/bin’, in the ‘ls’ example above, is one of the directories in ‘PATH’): $ echo $PATH /usr/local/sbin:/usr/local/bin:/usr/bin By default ‘PATH’ usually contains system-wide directories, which are readable (but not writable) by all users, like the above example. Therefore if you don’t have root (or administrator) access, you need to add another directory to ‘PATH’ which you actually have write access to. The standard directory where you can keep installed files (not just executables) for your own user is the ‘~/.local/’ directory. The names of hidden files start with a ‘<.>’ (dot), so it will not show up in your common command-line listings, or on the graphical user interface. You can use any other directory, but this is the most recognized. The top installation directory will be used to keep all the package’s components: programs (executables), libraries, include (header) files, shared data (like manuals), or configuration files. So it commonly has some of the following sub-directories for each class of components respectively: ‘bin/’, ‘lib/’, ‘include/’ ‘man/’, ‘share/’, ‘etc/’. Since the ‘PATH’ variable is only used for executables, you can add the ‘~/.local/bin’ directory to ‘PATH’ with the following command. As defined below, first the existing value of ‘PATH’ is used, then your given directory is added to its end and the combined value is put back in ‘PATH’ (run ‘‘$ echo $PATH’’ afterwards to check if it was added). $ PATH=$PATH:~/.local/bin Any executable that you installed in this directory will now be usable without having to remember and type its full address. However, as soon as you leave your current terminal session, this modification will be lost. Adding your specified directory to the ‘PATH’ environment variable each time you start a terminal is also very inconvenient and prone to errors. So there are standard ‘startup files’ defined by your shell. There is a special startup file for every significant starting step: ‘/etc/profile’ and everything in ‘/etc/profile.d/’ These startup scripts are called when your whole system starts (for example after you turn on your computer). Therefore you need administrator or root privileges to access or modify them. ‘~/.bash_profile’ If you are using (GNU) Bash as your shell, the commands in this file are run once every time you log in to your account. ‘~/.bashrc’ If you are using (GNU) Bash as your shell, the commands here will be run each time you start a terminal (for example, when you open your terminal emulator in the graphic user interface). For security reasons, it is highly recommended to directly type in your ‘HOME’ directory value by hand in startup files instead of using variables. So in the following, let’s assume your user name is ‘‘name’’. To add ‘~/.local/bin’ to your ‘PATH’ automatically on every startup you have to “export†the new value of ‘PATH’ in the startup file that is most relevant to you with the line ‘‘export PATH=$PATH:/home/name/.local/bin’’. You can either do it manually using a text editor, or by running the following command which will add this line as the last line of the file. Let’s assume you want to add it to ‘~/.bashrc’ (afterwards, open your ‘~/.bashrc’ with a text editor and check it out to see for your self): $ echo 'export PATH=$PATH:/home/name/.local/bin' >> ~/.bashrc Now that you know your system will look into ‘~/.local/bin’ for executables, you can tell Gnuastro’s configure script to install everything in the top ‘~/.local’ directory using the ‘--prefix’ option. The configure script will then put the executables in ‘~/.local/bin’, the compiled library files in ‘~/.local/lib’, the library header files in ‘~/.local/include’ and so on (see *note Review of library fundamentals:: for a review of the compiled library files and the headers). When you subsequently run ‘$ make install’, all the install-able files will be put in their respective directory under ‘~/.local/’ (as discussed above). Note that tilde (‘<~>’) expansion will not happen if you put a ‘<=>’ between ‘--prefix’ and ‘~/.local’(3), so we have avoided it here, see *note Options::. $ ./configure --prefix ~/.local You can install everything (including libraries like GSL, CFITSIO, or WCSLIB) locally by configuring them as above. However, recall that ‘PATH’ is only for executable files, not libraries. Therefore, when building programs or libraries(4) that depend on libraries you installed like this, you have to guide your compiler to the necessary directories. To do that, you have to define the ‘LDFLAGS’ and ‘CPPFLAGS’ environment variables respectively. This can be done while calling ‘./configure’: $ ./configure LDFLAGS=-L/home/name/.local/lib \ CPPFLAGS=-I/home/name/.local/include \ --prefix ~/.local It can be annoying to do this when configuring every package, so you can define these two variables in a startup file (discussed above). The convention on using these variables doesn’t include a colon to separate values (as ‘PATH’-like variables do), they use white space characters and each value is prefixed with a compiler option(5) (note the ‘-L’ and ‘-I’ above, see *note Options::). Therefore we have to keep the value in double quotation signs to keep the white space characters. Run the following two commands to do that if you want them in your ‘~/.bashrc’. echo 'export LDFLAGS="$LDFLAGS -L/home/name/.local/lib"' >> ~/.bashrc echo 'export CPPFLAGS="$CPPFLAGS -I/home/name/.local/include"' \ >> ~/.bashrc To be able to link to the locally installed dynamic libraries (which are linked at run time) after installation, add ‘~/.local/lib’ to your ‘LD_LIBRARY_PATH’ environment variable similar to the example above for ‘PATH’. If you also want to access the Info (see *note Info::) and man pages (see *note Man pages::) documentations add ‘~/.local/share/info’ and ‘~/.local/share/man’ to your ‘INFOPATH’(6) and ‘MANPATH’ environment variables. A final note is that order matters in the directories that are searched for all the variables discussed above. In the examples above, the new directory was added after the system specified directories. So if the program, library or manuals are found in the system wide directories, the user directory is no longer searched. If you want to search your local installation first, put the new directory before the already existing list like the example below. export LD_LIBRARY_PATH=/home/name/.local/lib:$LD_LIBRARY_PATH This is good when a library, for example CFITSIO, is already present on the system, but the system-wide install wasn’t configured with the correct configuration flags (see *note CFITSIO::), or you want to use a newer version and you don’t have administrator or root access to update it. With e above order ‘LD_LIBRARY_PATH’, the system will first find the CFITSIO you installed for yourself and will never reach the system-wide installation. However there are important security problems: because all important system-wide programs and libraries can be replaced by non-secure versions if they also exist in ‘./.local/’. So if you choose this order, be sure to keep it clean from executables or libraries with the same names as important system programs or libraries. ---------- Footnotes ---------- (1) By running ‘$ export myvariable=a_test_value’ instead of the simpler case in the text (2) You can use shell variables for other actions too, for example to temporarily keep some names or run loops on some files. (3) If you insist on using ‘<=>’, you can use ‘--prefix=$HOME/.local’. (4) For example WCSLIB which needs CFITSIO, or Gnuastro which needs both. (5) These variables are ultimately used as options while building the programs, so every value has be an option name followed be a value as discussed in *note Options::. (6) Info has the following convention: “If the value of ‘INFOPATH’ ends with a colon [or it isn’t defined] ..., the initial list of directories is constructed by appending the build-time default to the value of ‘INFOPATH’.†So when installing in a non-standard directory and if ‘INFOPATH’ was not initially defined, add a colon to the end of ‘INFOPATH’ as shown below, otherwise Info will not be able to find system-wide installed documentation: ‘echo 'export INFOPATH=$INFOPATH:/home/name/.local/share/info:' >> ~/.bashrc’ Note that this is only an internal convention of Info, do not use it for other ‘*PATH’ variables.  File: gnuastro.info, Node: Executable names, Next: Configure and build in RAM, Prev: Installation directory, Up: Configuring 3.3.1.3 Executable names ........................ At first sight, the names of the executables for each program might seem to be uncommonly long, for example ‘astnoisechisel’ or ‘astimgcrop’. We could have chosen terse (and cryptic) names like most programs do. We chose this complete naming convention (something like the commands in TeX) so you don’t have to spend too much time remembering what the name of a specific program was. Such complete names also enable you to easily search for the programs. To facilitate typing the names in, we suggest using the shell auto-complete. With this facility you can find the executable you want very easily. It is very similar to file name completion in the shell. For example, simply by typing the letters below (where <[TAB]> stands for the Tab key on your keyboard) $ ast[TAB][TAB] you will get the list of all the available executables that start with ‘ast’ in your ‘PATH’ environment variable directories. So, all the Gnuastro executables installed on your system will be listed. Typing the next letter for the specific program you want along with a Tab, will limit this list until you get to your desired program. In case all of this does not convince you and you still want to type short names, some suggestions are given below. You should have in mind though, that if you are writing a shell script that you might want to pass on to others, it is best to use the standard name because other users might not have adopted the same customizations. The long names also serve as a form of documentation in such scripts. A similar reasoning can be given for option names in scripts: it is good practice to always use the long formats of the options in shell scripts, see *note Options::. The simplest solution is making a symbolic link to the actual executable. For example let’s assume you want to type ‘ic’ to run ImageCrop instead of ‘astimgcrop’. Assuming you installed Gnuastro executables in ‘/usr/local/bin’ (default) you can do this simply by running the following command as root: # ln -s /usr/local/bin/astimgcrop /usr/local/bin/ic In case you update Gnuastro and a new version of ImageCrop is installed, the default executable name is the same, so your custom symbolic link still works. The installed executable names can also be set using options to ‘$ ./configure’, see *note Configuring::. GNU Autoconf (which configures Gnuastro for your particular system), allows the builder to change the name of programs with the three options ‘--program-prefix’, ‘--program-suffix’ and ‘--program-transform-name’. The first two are for adding a fixed prefix or suffix to all the programs that will be installed. This will actually make all the names longer! You can use it to add versions of program names to the programs in order to simultaneously have two executable versions of a program. The third configure option allows you to set the executable name at install time using the SED program. SED is a very useful ‘stream editor’. There are various resources on the internet to use it effectively. However, we should caution that using configure options will change the actual executable name of the installed program and on every re-install (an update for example), you have to also add this option to keep the old executable name updated. Also note that the documentation or configuration files do not change from their standard names either. For example, let’s assume that typing ‘ast’ on every invocation of every program is really annoying you! You can remove this prefix from all the executables at configure time by adding this option: $ ./configure --program-transform-name='s/ast/ /'  File: gnuastro.info, Node: Configure and build in RAM, Prev: Executable names, Up: Configuring 3.3.1.4 Configure and build in RAM .................................. The configure and build process involves the creation, reading, and modification of a large number of files (input/output, or I/O). Therefore file I/O issues can directly affect the work of developers who need to configure and build Gnuastro numerous times. Some of these issues are listed below: • I/O will cause wear and tear on both the HDDs (mechanical failures) and SSDs (decreasing the lifetime). • Having the built files mixed with the source files can greatly affect backing up (synchronization) of source files (since it involves the management of a large number of small files that are regularly changed. Backup software can of course be configured to ignore the built files and directories. However, since the built files are mixed with the source files and can have a large variety, this will require a high level of customization. One solution to address both these problems is to use the tmpfs file system (https://en.wikipedia.org/wiki/Tmpfs). Any file in tmpfs is actually stored in the RAM (and possibly SAWP), not on HDDs or SSDs. The RAM is built for extensive and fast I/O. Therefore the large number of file I/Os associated with configuring and building will not harm the HDDs or SSDs. Due to the volatile nature of RAM, files in the tmpfs file-system will be permanently lost after a power-off. Since all configured and built files are derivative files (not files that have been directly written by hand) there is no problem in this and this feature can be considered as an automatic cleanup. The modern GNU C library (and thus the Linux kernel) define the ‘/dev/shm’ directory for this purpose (POSIX shared memory). So using GNU Build System’s ability to build in a separate directory (not necessarily in the source directory), we can configure and build the programs in ‘/dev/shm’ to benefit from the RAM. To simplify the process, Gnuastro comes with a ‘tmpfs-config-make’ script. This script will create a directory in the shared memory, and put a symbolic link to it (called ‘build’) in the top source directory (the backup/sync software therefore only needs to ignore this single link/file). The script will then internally change to that directory and configure and build (‘make -kjN’, where ‘N’ is the number of threads for a parallel build) Gnuastro in there. To benefit from this script, simply run the following command instead of ‘./configure’ and ‘make’: $ ./tmpfs-config-make After this script is finished, you can ‘‘cd build’’ and run other Make commands (for example, ‘‘make check’’, ‘‘make install’’, or ‘‘make pdf’’) from there. In Emacs, the command to be run with the ‘M-x compile’ command (by default: ‘make -k’) can be changed to ‘‘cd build; make -kjN’’, or ‘‘make -C build -kjN’’ (‘N’ is the number of threads; an integer $\geq1$). For subsequent builds (during development) the ‘M-x recompile’ command will also do all the building in the RAM while you modify the clean, and backed-up source files and make minimal/efficient use of your non-volatile HDD or SSD. This script can be used in any software which is configured and built using the GNU Build System. Just copy it in the top source directory of that software and run it from there. The default number of threads and location of the shared memory (‘/dev/shm’) are currently hard-coded within the script. If you need to change them, please open the script with a text editor and set their values manually.  File: gnuastro.info, Node: Tests, Next: A4 print book, Prev: Configuring, Up: Build and install 3.3.2 Tests ----------- After successfully building (compiling) the programs with the ‘$ make’ command you can check the installation before installing. To run the tests, run $ make check For every program some tests are designed to check some possible operations. Running the command above will run those tests and give you a final report. If everything is ok and you have built all the programs, all the tests should pass. In case any of the tests fail, please have a look at *note Known issues:: and if that still doesn’t fix your problem, look that the ‘./tests/test-suite.log’ file to see if the source of the error is something particular to your system or more general. If you feel it is general, please contact us because it might be a bug. Note that the tests of some programs depend on the outputs of other program’s tests, so if you have not installed them they might be skipped or fail. Prior to releasing every distribution all these tests are checked. If you have a reasonably modern terminal, the outputs of the successful tests will be colored green and the failed ones will be colored red. These scripts can also act as a good set of examples for you to see how the programs are run. All the tests are in the ‘tests/’ directory. The tests for each program are shell scripts (ending with ‘.sh’) in a sub-directory of this directory with the same name as the program. See *note Test scripts:: for more detailed information about these scripts in case you want to inspect them.  File: gnuastro.info, Node: A4 print book, Next: Known issues, Prev: Tests, Up: Build and install 3.3.3 A4 print book ------------------- The default print version of this book is provided in the letter paper size. If you would like to have the print version of this book on paper and you are living in a country which uses A4, then you can rebuild the book. The great thing about the GNU build system is that the book source code which is in Texinfo is also distributed with the program source code, enabling you to do such customizations (hacking). In order to change the paper size, you will need to have GNU Texinfo installed. Open ‘doc/gnuastro.texi’ with any text editor. This is the source file that created this book. In the first few lines you will see this line: @c@afourpaper In Texinfo, a line is commented with ‘@c’. Therefore, un-comment this line by deleting the first two characters such that it changes to: @afourpaper Save the file and close it. You can now run $ make pdf and the new PDF book will be available in ‘SRCdir/doc/gnuastro.pdf’. By changing the ‘pdf’ in ‘$ make pdf’ to ‘ps’ or ‘dvi’ you can have the book in those formats. Note that you can do this for any book that is in Texinfo format, they might not have ‘@afourpaper’ line, so you can add it close to the top of the Texinfo source file.  File: gnuastro.info, Node: Known issues, Prev: A4 print book, Up: Build and install 3.3.4 Known issues ------------------ Depending on your operating system and the version of the compiler you are using, you might confront some known problems during the configuration (‘$ ./configure’), compilation (‘$ make’) and tests (‘$ make check’). Here, their solutions are discussed. • ‘$ ./configure’: _Configure complains about not finding a library even though you have installed it._ The possible solution is based on how you installed the package: • From your distribution’s package manager. Most probably this is because your distribution has separated the header files of a library from the library parts. Please also install the ‘development’ packages for those libraries too. Just add a ‘-dev’ or ‘-devel’ to the end of the package name and re-run the package manager. This will not happen if you install the libraries from source. When installed from source, the headers are also installed. • From source. Then your linker is not looking where you installed the library. If you followed the instructions in this chapter, all the libraries will be installed in ‘/usr/local/lib’. So you have to tell your linker to look in this directory. To do so, add ‘LDFLAGS=-L/usr/local/lib’ to the Gnuastro configure script. If you want to use the libraries for your other programming projects, then export this environment variable similar to the case for ‘LD_LIBRARY_PATH’ explained below. • ‘$ make’: _Complains about an unknown function on a non-GNU based operating system._ In this case, please run ‘$ ./configure’ with the ‘--enable-gnulibcheck’ option to see if the problem is from the GNU Portability Library (Gnulib) not supporting your system or if there is a problem in Gnuastro, see *note Gnuastro configure options::. If the problem is not in Gnulib and after all its tests you get the same complaint from ‘make’, then please contact us at ‘bug-gnuastro@gnu.org’. The cause is probably that a function that we have used is not supported by your operating system and we didn’t included it along with the source tar ball. If the function is available in Gnulib, it can be fixed immediately. • ‘$ make’: _Can’t find the headers (.h files) of libraries installed from source._ Similar to the case for ‘LDFLAGS’ (above), your compiler is not looking in the right place, add ‘CPPFLAGS=-I/usr/local/include’ to ‘./configure’ to re-configure Gnuastro, then re-run make. • ‘$ make check’: _Complaint about ‘rpl_malloc’ before the tests begin._ This is a problem with the different ways different operating systems implement C’s ‘malloc’ function. It doesn’t happen when building Gnuastro with ‘$ make’ because the GNU Portability Library (Gnulib) is used to compensate for the differences. But in ‘make check’, Gnulib is not used, so this error might pop-up there. To fix it, please re-run configure like below (adding any other options/arguments you might have already used): ./configure ac_cv_func_malloc_0_nonnull=yes • ‘$ make check’: _Only one ‘.sh’ test passes, all the rest fail._ It is highly likely that your distribution doesn’t look into the ‘/usr/local/lib’ directory when searching for shared libraries. To make sure it is added to the list of directories, run the following command and restart your terminal: (you can ignore the ‘\’ and extra space if you type it, it is only necessary if you copy and paste). See *note Installation directory:: for more details. echo 'export LD_LIBRARY_PATH=$LD_LIBRARY_PATH:/usr/local/lib' \ >> ~/.bashrc • ‘$ make check’: _The tests relying on external programs (for example ‘fitstopdf.sh’ fail._) This is probably due to the fact that the version number of the external programs is too old for the tests we have preformed. Please update the program to a more recent version. For example to create a PDF image, you will need GPL Ghostscript, but older versions do not work, we have successfully tested it on version 9.15. Older versions might cause a failure in the test result. • ‘$ make pdf’: _The PDF book cannot be made._ To make a PDF book, you need to have the GNU Texinfo program (like any program, the more recent the better). A working TeX program is also necessary, which you can get from Tex Live(1). • After ‘make check’: do not copy the programs’ executables to another (for example, the installation) directory manually (using ‘cp’, or ‘mv’ for example). In the default configuration(2), the program binaries need to link with Gnuastro’s shared library which is also built and installed with the programs. Therefore, to run successfully before and after installation, linking modifications need to be made by GNU Libtool at installation time. ‘make install’ does this internally, but a simple copy might give linking errors when you run it. If you need to copy the executables, you can do so after installation. If your problem was not listed above, please file a bug report (*note Report a bug::). ---------- Footnotes ---------- (1) (2) If you configure Gnuastro with the ‘--disable-shared’ option, then the libraries will be statically linked to the programs and this problem won’t exist, see *note Linking::.  File: gnuastro.info, Node: Common program behavior, Next: Extensions and Tables, Prev: Installation, Up: Top 4 Common program behavior ************************* There are some facts that are common to all the programs in Gnuastro which are mainly to do with user interaction. In this chapter these aspects are discussed. The most basic are the command-line options which are common in all the programs for a unified user experience. All Gnuastro programs can use configuration files so you don’t have to specify all the parameters on the command-line each time you run a program. The manner of setting, checking and using the these files at various levels are also explained. Finally we discuss how you can get immediate and distraction-free (without taking your hands off the keyboard!) help on the command-line. * Menu: * Command-line:: How to use the command-line. * Configuration files:: Values for unspecified variables. * Threads in Gnuastro:: How threads are managed in Gnuastro. * Final parameter values:: The final set of used parameters. * Automatic output:: About automatic output names. * Getting help:: Getting more information on the go. * Output headers:: Common headers to all FITS outputs.  File: gnuastro.info, Node: Command-line, Next: Configuration files, Prev: Common program behavior, Up: Common program behavior 4.1 Command-line ================ All the programs in Gnuastro are customized through the standard GNU style command-line options. First a general outline of how to make best use of these options is discussed and finally the options that are common to all the programs in Gnuastro are listed. Your full command-line text is passed onto the shell as a string of characters. That string is then broken up into separate ‘words’ by any ‘metacharacters’ (like space, tab, ‘|’, ‘>’ or ‘;’) that might exist in the text. See the GNU Bash manual, for the complete list of meta-characters and other Bash definitions. Its “Shell Operation†section has a short summary of the steps the shell takes before passing the commands to the program you called. * Menu: * Arguments and options:: Basics of options and arguments. * Arguments:: Treatment of arguments. * Options:: How to use GNU style options. * Common options:: Common options to all Gnuastro programs.  File: gnuastro.info, Node: Arguments and options, Next: Arguments, Prev: Command-line, Up: Command-line 4.1.1 Arguments and options --------------------------- On the command-line, the first thing you enter is the name of the program you want to run. After that you can specify two types of input: _arguments_ and _options_. Arguments are those tokens that are not preceded by any hyphens (‘-’), the program is suppose to understand what they are without any help from the user. Arguments can be both mandatory and optional and since there is no help from you, their order might also matter (for example in ‘cp’ which is used for copying). The outputs of ‘--usage’ and ‘--help’ shows which arguments are optional and which are mandatory, see *note --usage::. As their name suggests, _options_ are only optional and most of the time you don’t have to worry about what order you specify them in. In case your arguments or option values contain any of the shell’s meta-characters, you have to quote them. If there is only one such character, you can use a backslash (‘\’) before it. If there are multiple, it might be easier to simply put your whole argument or option value inside of double quotes (‘"’). In such cases, everything inside the double quotes will be seen as one ‘word’. For example let’s say you want to specify the Header data unit (HDU) of your FITS file using a complex expression like ‘3; images(exposure > 100)’. If you simply add these after the ‘--hdu’ (‘-h’) option, the programs in Gnuastro will read the value to the HDU option as ‘3’ and run. Then, Bash will attempt to run a separate command ‘images(exposure > 100)’ and complain about a syntax error. This is because the semicolon (‘;’) is an ‘end of command’ character in Bash. To solve this problem you can simply put double quotes around the whole string you want to pass as seen below: $ astimgcrop --hdu="3; images(exposure > 100)" FITSimage.fits Alternatively you can put a ‘\’ before every metacharacter in this string, but probably you will agree with us that the double quotes are much more easier, elegant and readable.  File: gnuastro.info, Node: Arguments, Next: Options, Prev: Arguments and options, Up: Command-line 4.1.2 Arguments --------------- In Gnuastro, the names of the input data files and ASCII tables are mostly specified as arguments, you can generally specify them in any order unless otherwise stated for a particular program. Everything particular about how a program treats arguments, is explained under the “Invoking ProgramName†section for that program. Generally, if there is a standard file name extension for a particular format, that filename extension is used to separate the kinds of arguments. The list below shows what astronomical data formats are recognized based on their file name endings. If the program doesn’t accept any other data format, any other argument that doesn’t end with the specified extensions below is considered to be a text file (usually catalogs). For example *note ConvertType:: accepts other data formats. • ‘.fits’: The standard file name ending of a FITS image. • ‘.fits.Z’: A FITS image compressed with ‘compress’. • ‘.fits.gz’: A FITS image compressed with GNU zip (gzip). • ‘.fits.fz’: A FITS image compressed with ‘fpack’. • ‘.imh’: IRAF format image file. Through out this book and in the command-line outputs, whenever we want to generalize all such astronomical data formats in a text place holder, we will use ‘ASTRdata’, we will assume that the extension is also part of this name. Any file ending with these names is directly passed on to CFITSIO to read. Therefore you don’t necessarily have to have these files on your computer, they can also be located on an FTP or HTTP server too, see the CFITSIO manual for more information. CFITSIO has its own error reporting techniques, if your input file(s) cannot be opened, or read, those errors will be printed prior to the final error by Gnuastro.  File: gnuastro.info, Node: Options, Next: Common options, Prev: Arguments, Up: Command-line 4.1.3 Options ------------- Command-line options allow configuring the behavior of a program in all GNU/Linux applications for each particular execution. Most options can be called in two ways: _short_ or _long_ a small number of options in some programs only have the latter type. In the list of options provided in *note Common options:: or those for each program, both formats are shown for those which support both. First the short is shown then the long. Short options are only one character and only have one hyphen (for example ‘-h’) while long options have two hyphens an can have many characters (for example ‘--hdu’). Usually, the short options are for when you are writing on the command line and want to save keystrokes and time. The long options are good for shell scripts, where you don’t usually have a rush and they provide a level of documentation, since they are less cryptic. Usually after a few months of not running a program, the short options will be forgotten and reading your previously written script will not be easy. Some options need to be given a value if they are called and some don’t. You can think of the latter type of options as on/off options. These two types of options can be distinguished using the output of the ‘--help’ and ‘--usage’ options, which are common to all GNU software, see *note Getting help::. The following convention is used for the formats of the values in Gnuastro: ‘INT’ The value is read as an integer. If a float or a string is provided the program will warn you and abort. In most cases, integers are used for counting variables, so if they are negative the program will also abort. ‘4or8’ Either the value 4 or 8, any other integer will give a warning and abort. ‘FLT’ The value is read as a float. There are generally two types, depending on the context. If they are for fractions, they will have to be less than or equal to unity. ‘STR’ The value is read as a string of characters (for example a file name) or other particular settings like a HDU name, see below. To specify a value in the short format, simply put the value after the option. Note that since the short options are only one character long, you don’t have to type anything between the option and its value. For the long option you either need white space or an ‘=’ sign, for example ‘-h2’, ‘-h 2’, ‘--hdu 2’ or ‘--hdu=2’ are all equivalent. The short format of on/off options (those that don’t need values) can be concatenated for example these two hypothetical sequences of options are equivalent: ‘-a -b -c4’ and ‘-abc4’. As an example, consider the following command to run ImageCrop: $ astimgcrop -Dr3 --wwidth 3 catalog.txt --deccol=4 ASTRdata The ‘$’ is the shell prompt, ‘astimgcrop’ is the program name. There are two arguments (‘catalog.txt’ and ‘ASTRdata’) and four options, two of them given in short format (‘-D’, ‘-r’) and two in long format (‘--width’ and ‘--deccol’). Three of them require a value and one (‘-D’) is an on/off option. If an abbreviation is unique between all the options of a program, the long option names can be abbreviated. For example, instead of typing ‘--printparams’, typing ‘--print’ or maybe even ‘--pri’ will be enough, if there are conflicts, the program will warn you and show you the alternatives. Finally, if you want the argument parser to stop parsing arguments beyond a certain point, you can use two dashes: ‘--’. No text on the command-line beyond these two dashes will be parsed. If an option with a value is repeated or called more than once, the value of the last time it was called will be assigned to it. This very useful in complicated situations, for example in scripts. Let’s say you want to make a small modification to one option value. You can simply type the option with a new value in the end of the command and see how the script works. If you are satisfied with the change, you can remove the original option. If the change wasn’t satisfactory, you can remove the one you just added and not worry about saving the original value. Without this capability, you would have to memorize or save the original value somewhere else, run the command and then change the value again which is not at all convenient and is potentially cause lots of bugs. When you don’t call an option that requires a value, all the programs in Gnuastro will check configuration files to find a value for that parameter. To learn more about how folder, user and system wide configuration files can be set, please see *note Configuration files::. Another factor that is particular to Gnuastro is that it will check the value you have given for each option to see if it is reasonable. For example you might mistakenly give a negative, float or string value for a FITS image extension or column number. As another example, you might give a value larger than unity for an option that only accepts fractions (which are always less than unity and positive). *CAUTION:* In specifying a file address, if you want to use the shell’s tilde expansion (‘~’) to specify your home directory, leave at least one space between the option name and your value. For example use ‘-o ~/test’, ‘--output ~/test’ or ‘--output= ~/test’. Calling them with ‘-o~/test’ or ‘--output=~/test’ will disable shell expansion. *CAUTION:* If you forget to specify a value for an option which requires one, and that option is the last one, Gnuastro will warn you. But if it is in the middle of the command, it will take the text of the next option or argument as the value which can cause undefined behavior. *NOTE:* All counting in Gnuastro starts from 0 not 1. So for example the first FITS image extension or column in a table are noted by 0, not 1. This is the standard in C and all languages that are based on it (for example C++, Java and Python).  File: gnuastro.info, Node: Common options, Prev: Options, Up: Command-line 4.1.4 Common options -------------------- To facilitate the job of the users and developers, all the programs in Gnuastro share some basic command-line options for the same operations where they are relevant. The list of options is provided below. It is noteworthy that these similar options are hard-wired into the programming of all of Gnuastro programs using GNU C library’s argument parser merging ability. For some programs, some of the options, might be irrelevant for example MakeProfiles creates FITS images based on a given catalog. Therefore no input images (and thus HDUs) are necessary for it. In such cases, the option is still listed and if a value is given for it, it is completely ignored. * Menu: * Input output:: Common input/output options. * Operating modes:: Common operating mode options.  File: gnuastro.info, Node: Input output, Next: Operating modes, Prev: Common options, Up: Common options 4.1.4.1 Input/Output options ............................ These options are to do with the input and outputs of the various programs. ‘-h’ ‘--hdu’ (‘=STR’) The number or name of the desired Header Data Unit or HDU in the input FITS image or images. A FITS file can store multiple HDUs or extensions, each with either an image or a table or nothing at all (only a header). Note that counting of the extensions starts from 0(zero), not 1(one). When specifying the name, case is not important so ‘IMAGE’, ‘image’ or ‘ImAgE’ are equivalent. A ‘#’ is appended to the string you specify for the HDU(1) and the result is put in square brackets and appended to the FITS file name before calling CFITSIO to read the contents of the HDU for all the programs in Gnuastro. CFITSIO has many capabilities to help you find the extension you want, far beyond the simple extension number and name. See CFITSIO manual’s “HDU Location Specification†section for a very complete explanation with several examples. Note that in some programs, the behavior of ‘--hdu’ might be different, for example see *note Invoking astarithmetic::, were it can be called multiple times and the value of each all will be stored. ‘-o’ ‘--output’ (‘=STR’) The name of the output file or directory. With this option the automatic output names explained in *note Automatic output:: are ignored. ‘-D’ ‘--dontdelete’ By default, if the output file already exists, it will be silently replaced with the output of this run of all Gnuastro programs. By calling this option, if the output file already exists, the programs will warn you and abort. ‘-K’ ‘--keepinputdir’ In automatic output names, don’t remove the directory information of the input file names. As explained in *note Automatic output::, if no output name is specified, then the output name will be made in the existing directory based on your input. If you call this option, the directory information of the input will be kept and the output will be in the same directory as the input. Note that his is only relevant if you are running the program from another directory! ---------- Footnotes ---------- (1) With the ‘#’ character, CFITSIO will only read the desired HDU into your memory, not all the existing HDUs in the fits file.  File: gnuastro.info, Node: Operating modes, Prev: Input output, Up: Common options 4.1.4.2 Operating modes ....................... Another group of options that are common to all the programs in Gnuastro are those to do with the general operation of the programs. The explanation for those that are not only limited to Gnuastro but can be called in all GNU programs start with (GNU option). ‘--’ (GNU option) Stop parsing the command-line. This option can be useful in scripts or when using the shell history. Suppose you have a long list of options, and want to see if removing some of them (and using the default values) can give a better result. If the ones you want to remove are the last ones on the command-line, you don’t have to delete them, you can just add ‘--’ before them and if you don’t get what you want, you can remove the ‘--’ and get the same initial result. ‘--usage’ (GNU option) Only print the options and arguments. This is very useful for when you know the what the options do, you have just forgot their names. See *note --usage::. ‘-?’ ‘--help’ (GNU option) Print all options and an explanation. Adding this option will print all the options in their short and long formats, also displaying which ones need a value if they are called (with an ‘=’ after the long format). A short explanation is also given for what the option is for. The program will quit immediately after the message is printed and will not do any form of processing. See *note --help::. ‘-V’ ‘--version’ (GNU option) Print a short message, showing the full name, version, copyright information and program authors. On the first line it will print the official name (not executable name) and version number of the program. It will also print the version of the Gnuastro that the program was built with. Following this is a blank line and a copyright information. The program will not run. ‘-q’ ‘--quiet’ Don’t report steps. All the programs in Gnuastro that have multiple major steps will report their steps for you to follow while they are operating. If you do not want to see these reports, you can call this option and only error messages will be printed if the program is aborted. If the steps are done very fast (depending on the properties of your input) disabling these reports will also decrease running time. ‘--cite’ Print the BibTeX entry for Gnuastro and the particular program (if that program comes with a separate paper) and abort. Citations are vital for the continued work on Gnuastro. Gnuastro started and is continued based on separate research projects. So if you find any of the tools offered in Gnuastro to be useful in your research, please use the output of this command to cite the program and Gnuastro in your research paper. Thank you. Gnuastro is still new, there is no separate paper only devoted to Gnuastro yet. Therefore currently the paper to cite for Gnuastro is the paper for NoiseChisel which is the first published paper introducing Gnuastro to the astronomical community. Upon reaching a certain point, a paper completely devoted to Gnuastro will be published, see *note GNU Astronomy Utilities 1.0::. ‘-P’ ‘--printparams’ Print the final values used for all the parameters and abort. See *note Final parameter values:: for more details. ‘-S’ ‘--setdirconf’ Update the current directory configuration file from the given command line options and quit, see *note Configuration files::. The values of your options are added to the configuration file in the current directory. If the configuration file or folder doesn’t exist, it will be created. If it exists but has different values for those options, they will be given the new values. In any case, the program will not run, but the contents of its updated configuration file are printed for you to inspect. This is the recommended method to fill the configuration file for all future calls to one of the Gnuastro programs in a folder. It will internally check if your values are in the correct range and type and save them according to the configuration file format, see *note Configuration file format::. When this option is called, the otherwise mandatory arguments, for example input image or catalog file(s), are no longer mandatory (since the program will not run). ‘-U’ ‘--setusrconf’ Update the user configuration file from the command-line options and quit. See explanation under ‘--setdirconf’ for more details. ‘--onlydirconf’ Only read the current (local) directory configuration file and ignore the rest of the configuration files, see *note Configuration file precedence:: and *note Current directory and User wide::. This can be very useful when you want your results to be exactly reproducible. All the configuration files can be put in the hidden ‘./.gnuastro/’ directory in the current directory, or the hidden directory can be a symbolic link to the directory containing the configuration files. Then with this option you can ensure that no other configuration file is read. So if your local configuration file lacks some parameters, which ever Gnuastro program you are using will will warn you and abort, enabling you to exactly set all the necessary parameters without unknowingly relying on some user or system wide option values. ‘onlydirconf’ can also be used in the configuration files (with a value of ‘0’ or ‘1’), see *note Configuration file format::. If it is present in the local configuration file, other configuration files will not be read. In the other configuration files, it is irrelevant. ‘--onlyversion’ (‘=STR’) Only run the program if its version is equal with the string of characters given to this option. Note that it is not compared as a number, but as a string of characters, so ‘0’, or ‘0.0’ and ‘0.00’ are different. This is useful if you want your results to be exactly reproducible and not mistakenly run with an updated or older version of the program. ‘--nolog’ For programs which generate Log files, if this option is called, no Log file will be generated. ‘-N’ ‘--numthreads’ (‘=INT’) Set the number of CPU threads to use. See *note Threads in Gnuastro::.  File: gnuastro.info, Node: Configuration files, Next: Threads in Gnuastro, Prev: Command-line, Up: Common program behavior 4.2 Configuration files ======================= Each program needs a certain number of parameters to run. Supplying all the necessary parameters each time you run the program is very frustrating and prone to errors. Therefore all the programs read the values for the necessary options you have not given in the command line from one of several plain text files (which you can view and edit with any text editor). These files are known as configuration files and are usually kept in a directory named ‘etc/’ according to the file system hierarchy standard(1). The thing to have in mind is that none of the programs in Gnuastro keep any internal default value. All the values must either be stored in one of the configuration files or explicitly called in the command-line. In case the necessary parameters are not given through any of these methods, the program will list the missing necessary parameters and abort. The only exception to this is ‘--numthreads’, whose default value is determined at run-time using the number of threads available to your system, see *note Threads in Gnuastro::. Of course, you can still provide a default value for the number of threads at any of the levels below, but if you don’t, the program will not abort. Also note that through automatic output name generation, the value to the ‘--output’ option is also not mandatory on the command-line or in the configuration files for all programs which don’t rely on that value as an input(2), see *note Automatic output::. * Menu: * Configuration file format:: ASCII format of configuration file. * Configuration file precedence:: Precedence of configuration files. * Current directory and User wide:: Local and user configuration files. * System wide:: System wide configuration files. ---------- Footnotes ---------- (1) (2) One example of a program which uses the value given to ‘--output’ as an input is ConvertType, this value specifies the type of the output through the value to ‘--output’, see *note Invoking astconvertt::.  File: gnuastro.info, Node: Configuration file format, Next: Configuration file precedence, Prev: Configuration files, Up: Configuration files 4.2.1 Configuration file format ------------------------------- The configuration files for each program have the standard program executable name with a ‘.conf’ suffix. When you download the source code, you can find them in the same directory as the source code of each program, see *note Program source::. Any line in the configuration file whose first non-white character is a <#> is considered to be a comment and is ignored. The same goes for an empty line. The name of the parameter is the same as the long format of the command-line option for that parameter. The parameter name and parameter value have to be separated by any number of ‘white-space’ characters: space, tab or vertical tab. By default several space characters are used. If the value of an option has space characters (most commonly for the ‘hdu’ option), then double quotes can be used to specify the full value. In each non-commented and non-blank line, any text after the first two words (given the conditions above) is ignored. If it is an option without a value in the ‘--help’ output (on/off option, see *note Options::), then the value should be ‘1’ if it is to be ‘on’ and ‘0’ otherwise. If an option is not recognized in the configuration file, the name of the file and unrecognized option will be reported and the program will abort. If a parameter is repeated more more than once in the configuration files and it is not set on the command-line, then only the first value will be used, the rest will be ignored. You can build or edit any of the directories and the configuration files yourself using any text editor. However, it is recommended to use the ‘--setdirconf’ and ‘--setusrconf’ options to set default values for the current directory or this user, see *note Operating modes::. With these options, the values you give will be checked as explained in *note Options:: before writing in the current directory’s configuration file. They will also print a set of commented lines guiding the reader and will also classify the options based on their context and write them in their logical order to be more understandable.  File: gnuastro.info, Node: Configuration file precedence, Next: Current directory and User wide, Prev: Configuration file format, Up: Configuration files 4.2.2 Configuration file precedence ----------------------------------- The parameter values in all the programs of Gnuastro will be filled in the following order. Such that if a parameter is assigned a value in an earlier step, any value for that parameter in a later step will be ignored. 1. Command-line options, for this particular execution. 2. Current directory, for all executions in the directory from which any of the programs is run (‘./.gnuastro/’). 3. The user’s home directory, for all the executions of a particular user: (‘$HOME/.local/etc/’, see below). It is only read if ‘--onlydirconf’ is not called, see *note Operating modes::. 4. In a system wide directory for any user on that computer (‘prefix/etc/’, see *note Installation directory:: for the value of ‘prefix’). It is only read if ‘--onlydirconf’ is not called, see *note Operating modes::. The basic idea behind setting this progressive state of checking for parameter values is that separate users of a computer or separate folders in a user’s file system might need different values for some parameters and the same values for others. For example raw telescope images usually have their main image extension in the second FITS extension, while processed FITS images usually only have one extension. If your system wide default input extension is 0 (the first), then when you want to work with the former group of data you have to explicitly mention it to the programs every time. With this progressive state of default values to check, you can set different default values for the different directories that you would like to run Gnuastro in for your different purposes, so you won’t have to worry about this issue any more.  File: gnuastro.info, Node: Current directory and User wide, Next: System wide, Prev: Configuration file precedence, Up: Configuration files 4.2.3 Current directory and User wide ------------------------------------- For the current (local) and user-wide directories, the configuration files are stored in the hidden sub-directories named ‘./.gnuastro/’ and ‘HOME/.local/etc/’ respectively. Unless you have changed it, the ‘HOME’ environment variable should point to your home directory. You can check it by running ‘$ echo $HOME’. Each time you run any of the programs in Gnuastro, this environment variable is read and placed in the above address. So if you suddenly see that your home configuration files are not being read, probably you (or some other program) has changed the value of this environment variable. Although it might cause confusions like above, this dependence on the ‘HOME’ environment variable enables you to temporarily use a different directory as your home directory. This can come in handy in complicated situations. To set the user or current directory configuration files based on your command-line input, you can use the ‘--setdirconf’ or ‘--setusrconf’, see *note Operating modes::  File: gnuastro.info, Node: System wide, Prev: Current directory and User wide, Up: Configuration files 4.2.4 System wide ----------------- When Gnuastro is installed, the configuration files that are shipped with the distribution are copied into the (possibly system wide) ‘prefix/etc/’ directory. See *note Configuring:: for more details on ‘prefix’ (by default it is: ‘/usr/local’). This directory is the final place (with the lowest priority) that the programs in Gnuastro will check to retrieve parameter values. If you remove a parameter and its value from the files in this system wide directory, you either have to specify it in more immediate configuration files or set it each time in the command-line. Recall that none of the programs in Gnuastro keep any internal default values and will abort if they don’t find a value for the necessary parameters (except the number of threads). So even though you might never use a parameter, it still has to be at least available in this system-wide configuration file. In case you install Gnuastro from your distribution’s repositories, ‘prefix’ will either be set to ‘/’ (the root directory) or ‘/usr’, so you can find the system wide configuration variables in ‘/etc/’ or ‘/usr/etc/’. The prefix of ‘/usr/local/’ is conventionally used for programs you install from source by your self.  File: gnuastro.info, Node: Threads in Gnuastro, Next: Final parameter values, Prev: Configuration files, Up: Common program behavior 4.3 Threads in Gnuastro ======================= Some of the programs benefit significantly when you use all the threads your computer’s CPU has to offer to your operating system. GNU Astronomy Utilities uses the POSIX threads library (pthreads) for spinning off threads when the user asks for it. The number of threads available to your operating system is usually double the number of physical (hardware) cores in your CPU. On a GNU/Linux system, the number of threads available can be found with the command ‘$ nproc’ command (part of GNU Coreutils). Gnuastro can find the number of threads available to your system at run-time (when you execute the program). However, if a value is given provided for the ‘--numthreads’ option, the given value will be used, not the value automatically read from your system, see *note Operating modes:: and *note Configuration files:: for ways to set a different value. Thus ‘--numthreads’ is the only option with a value that doesn’t have to be specified anywhere on the command-line or in the options. * Menu: * A note on threads:: Caution and suggestion on using threads. * How to run simultaneous operations:: How to run things simultaneously.  File: gnuastro.info, Node: A note on threads, Next: How to run simultaneous operations, Prev: Threads in Gnuastro, Up: Threads in Gnuastro 4.3.1 A note on threads ----------------------- Spinning off threads internally is not necessarily always the most efficient way to run an application. Creating a new thread isn’t a cheap operation for the operating system. It is most useful when the input data are fixed and you want the same operation to be done on parts of it. For example one input image to ImageCrop and multiple crops from various parts of it. In this fashion, the image is loaded into memory once, all the crops are divided between the number of threads internally and each thread cuts out those parts which are assigned to it from the same image. On the other hand, if you have multiple images and you want to crop the same region out of all of them, it is much more efficient to set ‘--numthreads=1’ (so no threads spin off) and run ImageCrop multiple times simultaneously, see *note How to run simultaneous operations::. You can check the boost in speed by first running a program on one of the data sets with the maximum number of threads and another time (with everything else the same) and only using one thread. You will notice that the wall-clock time (reported by most programs at their end) in the former is longer than the latter divided by number of physical CPU cores available to your operating system. Asymptotically these two can be equal (most of the time they aren’t). So limiting the programs to use only one thread and running them independently on the number of available threads will be more efficient. Note that the operating system keeps a cache of recently processed data, so usually, the second time you process an identical data set (independent of the number of threads used), you will get faster results. In order to make an unbiased comparison, you have to first clean the system’s cache with the following command between the two runs. $ sync; echo 3 | sudo tee /proc/sys/vm/drop_caches *SUMMARY: Should I use multiple threads?* Depends: • If you only have *one* data set (image in most cases!), then yes, the more threads you use (with a maximum of the number of threads available to your OS) the faster you will get your results. • If you want to run the same operation on *multiple* data sets, it is best to set the number of threads to 1 and use GNU Parallel as explained above.  File: gnuastro.info, Node: How to run simultaneous operations, Prev: A note on threads, Up: Threads in Gnuastro 4.3.2 How to run simultaneous operations ---------------------------------------- There are two approaches to simultaneously execute a program: using GNU Parallel or Make (GNU Make is the most common implementation). The first is very useful when you only want to do one job multiple times and want to get back to your work without actually keeping the command you ran. The second is usually for (very) complicated processes, with lots of dependencies between the different products (for example a data-production pipeline). GNU Parallel When you only want to run multiple instances of a command on different threads and get on with the rest of your work, the best method is to use GNU parallel. Surprisingly GNU Parallel is one of the few GNU packages that has no Info documentation but only a Man page, see *note Info::. So to see the documentation after installing it please run $ man parallel As an example, let’s assume we want to crop a region fixed on the pixels (500, 600) with the default width from all the FITS images in the ‘./data’ directory ending with ‘sci.fits’ to the current directory. To do this, you can run: $ parallel astimgcrop --numthreads=1 --xc=500 --yc=600 ::: \ ./data/*sci.fits GNU Parallel can help in many more conditions, this is one of the simplest, see the man page for lots of other examples. For absolute beginners: the backslash (‘\’) is only a line breaker to fit nicely in the page. If you type the whole command in one line, you should remove it. Make Make is a program built for specifying “targetsâ€, “prerequisites†and “recipesâ€. It allows you to define very complicated dependency structures for complicated processes that commonly start off with a large list of inputs and builds them based on the dependencies you define. GNU Make(1) is the most common implementation which (like nearly all GNU programs comes with a wonderful manual(2)). It is very basic and short (the most important part is about 100 pages). Make has the ‘--jobs’ (‘-j’) which allows you to specify the maximum number of jobs that can be done simultaneously. For example a common 4 physical core CPU usually has 8 processing threads. So you can run: $ make -j8 Once the dependency tree for your processes is built, Make will run the independent targets simultaneously. ---------- Footnotes ---------- (1) (2)  File: gnuastro.info, Node: Final parameter values, Next: Automatic output, Prev: Threads in Gnuastro, Up: Common program behavior 4.4 Final parameter values, reproduce previous results ====================================================== The input parameters can be specified in many places, either on the command-line or in at least one of several configuration files, see *note Configuration files::. Therefore, it often happens that before running a program on a certain data set, you want to see the values for the parameters that the program will use after it has read your command-line options and all the configuration files in their correct order. You might also want to save the list with the output so you can reproduce the same results at a later time, this is very important when you want to use your results in a report or paper. If you call the ‘--printparams’ option, all Gnuastro programs will read your command-line parameters and all the configuration files. If there is no problem (like a missing parameter or a value in the wrong format) and immediately before actually running, the programs will print the full list of parameter names and values sorted and grouped by context and quit. They will also report their version number, the date they were configured on your system and the time they were reported. As an example, you can give your full command-line options and even the input and output file names and finally just add ‘-P’ to check if all the parameters are finely set. If everything is ok, you can just run the same command (easily retrieved from the bash history, with the top arrow key) and simply remove the last two characters that showed this option. Since no program will actually start its processing when this option is called, the otherwise mandatory arguments for each program (for example input image or catalog files) are no longer required when you call this option. In case you want to store the list of parameters for later reproduction of the same results, you can do so with the GNU Bash re-direction tool. For example after you have produced the results you want to store, you can save all the parameters that were used in a file named ‘parameters.txt’ in the following manner. Using shell history you can retrieve the last command you entered and simply add ‘-P > parameters.txt’ to it, for example: $ astimgcrop --racol=2 --deccol=3 IN.fits cat.txt -P > parameters.txt All the parameters along with the extra data explained before will be stored in the plain text ‘parameters.txt’ file through the shell’s redirection mechanism (‘>’). The output of ‘--printparams’ conforms with the configuration file formats(1). By taking the following steps, you can use this file as a configuration file to reproduce your results at a later time. 1. Set the file name based on the standard configuration file names, see *note Configuration file format::. 2. Later on (when ever you want to re-produce your results), copy the file in the ‘./.gnuastro/’ directory of your current directory. In this manner, this file will be read as a current directory configuration file and since all the parameters are defined in it, no other configuration file value will be used. ---------- Footnotes ---------- (1) They are both written by the same function.  File: gnuastro.info, Node: Automatic output, Next: Getting help, Prev: Final parameter values, Up: Common program behavior 4.5 Automatic output ==================== All the programs in Gnuastro are designed such that specifying an output file or directory (based on the program context) is optional. The outputs of most programs are automatically found based on the input and what the program does. For example when you are converting a FITS image named ‘FITSimage.fits’ to a JPEG image, the JPEG image will be saved in ‘FITSimage.jpg’. Another very important part of the automatic output generation is that all the directory information of the input file name is stripped off of it. This feature can be disabled with the ‘--keepinputdir’ option, see *note Common options::. It is the default because astronomical data are usually very large and organized specially with special file names. In some cases, the user might not have write permissions in those directories. In fact, even if the data is stored on your own computer, it is advised to only grant write permissions to the super user or root. This way, you won’t accidentally delete or modify your valuable data! Let’s assume that we are working on a report and want to process the FITS images from two projects (ABC and DEF), which are stored in the sub-directories named ‘ABCproject/’ and ‘DEFproject/’ of our top data directory (‘/mnt/data’). The following shell commands show how one image from the former is first converted to a JPEG image through ConvertType and then the objects from an image in the latter project are detected using NoiseChisel. The text after the ‘#’ sign are comments (not typed!). $ pwd # Current location /home/usrname/research/report $ ls # List directory contents ABC01.jpg $ ls /mnt/data/ABCproject # Archive 1 ABC01.fits ABC02.fits ABC03.fits $ ls /mnt/data/DEFproject # Archive 2 DEF01.fits DEF02.fits DEF03.fits $ astconvertt /mnt/data/ABCproject/ABC02.fits --output=jpg # Prog 1 $ ls ABC01.jpg ABC02.jpg $ astnoisechisel /mnt/data/DEFproject/DEF01.fits # Prog 2 $ ls ABC01.jpg ABC02.jpg DEF01_labeled.fits  File: gnuastro.info, Node: Getting help, Next: Output headers, Prev: Automatic output, Up: Common program behavior 4.6 Getting help ================ Probably the first time you read this book, it is either in the PDF or HTML formats. These two formats are very convenient for when you are not actually working, but when you are only reading. Later on, when you start to use the programs and you are deep in the middle of your work, some of the details will inevitably be forgotten. Going to find the PDF file (printed or digital) or the HTML webpage is a major distraction. GNU software have a very unique set of tools for aiding your memory on the command-line, where you are working, depending how much of it you need to remember. In the past, such command-line help was known as “online†help, because they were literally provided to you ‘on’ the command ‘line’. However, nowadays the word “online†refers to something on the internet, so that term will not be used. With this type of help, you can resume your exciting research without taking your hands off the keyboard. Another major advantage of such command-line based help routines is that they are installed with the software in your computer, therefore they are always in sync with the executable you are actually running. Three of them are actually part of the executable. You don’t have to worry about the version of the book or program. If you rely on external help (a PDF in your personal print or digital archive or HTML from the official webpage) you have to check to see if their versions fit with your installed program. If you only need to remember the short or long names of the options, ‘--usage’ is advised. If it is what the options do, then ‘--help’ is a great tool. Man pages are also provided for those who are use to this older system of documentation. This full book is also available to you on the command-line in Info format. If none of these seems to resolve the problems, there is a mailing list which enables you to get in touch with experienced Gnuastro users. In the subsections below each of these methods are reviewed. * Menu: * --usage:: View option names and value formats. * --help:: List all options with description. * Man pages:: Man pages generated from –help. * Info:: View complete book in terminal. * help-gnuastro mailing list:: Contacting experienced users.  File: gnuastro.info, Node: --usage, Next: --help, Prev: Getting help, Up: Getting help 4.6.1 ‘--usage’ --------------- If you give this option, the program will not run. It will only print a very concise message showing the options and arguments. Everything within square brackets (‘[]’) is optional. For example here are the first and last two lines of ImageCrop’s ‘--usage’ is shown: $ astimgcrop --usage Usage: astimgcrop [-Do?IPqSVW] [-d INT] [-h INT] [-r INT] [-w INT] [-x INT] [-y INT] [-c INT] [-p STR] [-N INT] [--deccol=INT] .... [--setusrconf] [--usage] [--version] [--wcsmode] [ASCIIcatalog] FITSimage(s).fits There are no explanations on the options, just their short and long names shown separately. After the program name, the short format of all the options that don’t require a value (on/off options) is displayed. Those that do require a value then follow in separate brackets, each displaying the format of the input they want, see *note Options::. Since all options are optional, they are shown in square brackets, but arguments can also be optional. For example in this example, a catalog name is optional and is only required in some modes. This is a standard method of displaying optional arguments for all GNU software.  File: gnuastro.info, Node: --help, Next: Man pages, Prev: --usage, Up: Getting help 4.6.2 ‘--help’ -------------- If the command-line includes this option, the program will not be run. It will print a complete list of all available options along with a short explanation. The options are also grouped by their context. Within each context, the options are sorted alphabetically. Since the options are shown in detail afterwards, the first line of the ‘--help’ output shows the arguments and if they are optional or not, similar to *note --usage::. In the ‘--help’ output of all programs in Gnuastro, the options for each program are classified based on context. The first two contexts are always options to do with the input and output respectively. For example input image extensions or supplementary input files for the inputs. The last class of options is also fixed in all of Gnuastro, it shows operating mode options. Most of these options are already explained in *note Operating modes::. The help message will sometimes be longer than the vertical size of your terminal. If you are using a graphical user interface terminal emulator, you can scroll the terminal with your mouse, but we promised no mice distractions! So here are some suggestions: • to scroll up and to scroll down. For most help output this should be enough. The problem is that it is limited by the number of lines that your terminal keeps in memory and that you can’t scroll by lines, only by whole screens. • Pipe to ‘less’. A pipe is a form of shell re-direction. The ‘less’ tool in Unix-like systems was made exactly for such outputs of any length. You can pipe (‘|’) the output of any program that is longer than the screen to it and then you can scroll through (up and down) with its many tools. For example: $ astnoisechisel --help | less Once you have gone through the text, you can quit ‘less’ by pressing the key. • Redirect to a file. This is a less convenient way, because you will then have to open the file in a text editor! You can do this with the shell redirection tool (‘>’): $ astnoisechisel --help > filename.txt In case you have a special keyword you are looking for in the help, you don’t have to go through the full list. GNU Grep is made for this job. For example if you only want the list of options whose ‘--help’ output contains the word “axis†in ImageCrop, you can run the following command: $ astimgcrop --help | grep axis If the output of this option does not fit nicely within the confines of your terminal, GNU does enable you to customize its output through the environment variable ‘ARGP_HELP_FMT’, you can set various parameters which specify the formatting of the help messages. For example if your terminals are wider than 70 spaces (say 100) and you feel there is too much empty space between the long options and the short explanation, you can change these formats by giving values to this environment variable before running the program with the ‘--help’ output. You can define this environment variable in this manner: $ export ARGP_HELP_FMT=rmargin=100,opt-doc-col=20 This will affect all GNU programs using GNU C library’s ‘argp.h’ facilities as long as the environment variable is in memory. You can see the full list of these formatting parameters in the “Argp User Customization†part of the GNU C library manual. If you are more comfortable to read the ‘--help’ outputs of all GNU software in your customized format, you can add your customizations (similar to the line above, without the ‘$’ sign) to your ‘~/.bashrc’ file. This is a standard option for all GNU software.  File: gnuastro.info, Node: Man pages, Next: Info, Prev: --help, Up: Getting help 4.6.3 Man pages --------------- Man pages were the Unix method of providing command-line documentation to a program. With GNU Info, see *note Info:: the usage of this method of documentation is highly discouraged. This is because Info provides a much more easier to navigate and read environment. However, some operating systems require a man page for packages that are installed and some people are still used to this method of command line help. So the programs in Gnuastro also have Man pages which are automatically generated from the outputs of ‘--version’ and ‘--help’ using the GNU help2man program. So if you run $ man programname You will be provided with a man page listing the options in the standard manner.  File: gnuastro.info, Node: Info, Next: help-gnuastro mailing list, Prev: Man pages, Up: Getting help 4.6.4 Info ---------- Info is the standard documentation format for all GNU software. It is a very useful command-line document viewing format, fully equipped with links between the various pages and menus and search capabilities. As explained before, the best thing about it is that it is available for you the moment you need to refresh your memory on any command-line tool in the middle of your work without having to take your hands off the keyboard. This complete book is available in Info format and can be accessed from anywhere on the command-line. To open the Info format of any installed programs or library on your system which has an Info format book, you can simply run the command below (change ‘executablename’ to the executable name of the program or library): $ info executablename In case you are not already familiar with it, run ‘$ info info’. It does a fantastic job in explaining all its capabilities its self. It is very short and you will become sufficiently fluent in about half an hour. Since all GNU software documentation is also provided in Info, your whole GNU/Linux life will significantly improve. Once you’ve become an efficient navigator in Info, you can go to any part of this book or any other GNU software or library manual, no matter how long it is, in a matter of seconds. It also blends nicely with GNU Emacs (a text editor) and you can search manuals while you are writing your document or programs without taking your hands off the keyboard, this is most useful for libraries like the GNU C library. To be able to access all the Info manuals installed in your GNU/Linux within Emacs, type . To see this whole book from the beginning in Info, you can run $ info gnuastro If you run Info with the particular program executable name, for example ‘astimgcrop’ or ‘astnoisechisel’: $ info astprogramname you will be taken to the section titled “Invoking ProgramName†which explains the inputs and outputs along with the command-line options for that program. Finally, if you run Info with the official program name, for example ImageCrop or NoiseChisel: $ info ProgramName you will be taken to the top section which introduces the program. Note that in all cases, Info is not case sensitive.  File: gnuastro.info, Node: help-gnuastro mailing list, Prev: Info, Up: Getting help 4.6.5 help-gnuastro mailing list -------------------------------- Gnuastro maintains the help-gnuastro mailing list for users to ask any questions related to Gnuastro. The experienced Gnuastro users and some of its developers are subscribed to this mailing list and your email will be sent to them immediately. However, when contacting this mailing list please have in mind that they are possibly very busy and might not be able to answer immediately. To ask a question from this mailing list, send a mail to ‘help-gnuastro@gnu.org’. Anyone can view the mailing list archives at . It is best that before sending a mail, you search the archives to see if anyone has asked a question similar to yours. If you want to make a suggestion or report a bug, please don’t send a mail to this mailing list. We have other mailing lists and tools for those purposes, see *note Report a bug:: or *note Suggest new feature::.  File: gnuastro.info, Node: Output headers, Prev: Getting help, Up: Common program behavior 4.7 Output headers ================== The output FITS files created by Gnuastro’s programs have some or all of the following standard keywords to keep the basic date and version information of Gnuastro, its dependencies and the pipeline that is using Gnuastro. ‘DATE’ The creation time of the FITS file. This date is written directly by CFITSIO and is in UT format. ‘COMMIT’ Git’s commit description from the running directory of Gnuastro’s programs. If the running directory is not version controlled or ‘libgit2’ isn’t installed (see *note Optional dependencies::) then this keyword will not be present. The printed value is equivalent to the output of the following command: git describe --dirty --always If the running directory contains non-committed work, then the stored value will have a ‘‘-dirty’’ suffix. This can be very helpful to let you know that the data is not ready to be shared with collaborators or submitted to a journal. You should only share results that are produced after all your work is committed (safely stored in the version controlled history and thus reproducible). At first sight, version control appears to be mainly a tool for software developers. However progress in a scientific research is almost identical to progress in software development: first you have a rough idea that starts with handful of easy steps. But as the first results appear to be promising, you will have to extend, or generalize, it to make it more robust and work in all the situations your research covers, not just your first test samples. Slowly you will find wrong assumptions or bad implementations that need to be fixed (‘bugs’ in software development parlance). Finally, when you submit the research to your collaborators or a journal, many comments and suggestions will come in, and you have to address them. Software developers have created version control systems precisely for this kind of activity. Each significant moment in the project’s history is called a “commitâ€, see *note Version controlled source::. A snapshot of the project in each “commit†is safely stored away, so you can revert back to it at a later time, or check changes/progress. This way, you can be sure that your work is reproducible and track the progress and history. With version control, experimentation in the project’s analysis is greatly facilitated, since you can easily revert back if a brainstorm test procedure fails. One important feature of version control is that the research result (FITS image, table, report or paper) can be stamped with the unique commit information that produced it. This information will enable you to exactly reproduce that same result later, even if you have made changes/progress. For one example of a research paper’s reproduction pipeline, please see the reproduction pipeline (https://gitlab.com/makhlaghi/NoiseChisel-paper) of the paper (https://arxiv.org/abs/1505.01664) describing *note NoiseChisel::. ‘CFITSIO’ The version of CFITSIO used (see *note CFITSIO::). ‘WCSLIB’ The version of WCSLIB used (see *note WCSLIB::). Note that older versions of WCSLIB do not report the version internally. So this is only available if you are using more recent WCSLIB versions. ‘GNUASTRO’ The version of Gnuastro used (see *note Version numbering::). Here is one example of the last few lines of an example output. / Versions and date DATE = '...' / file creation date COMMIT = 'v0-8-g547f6eb' / Commit description in running dir. CFITSIO = '3.39 ' / CFITSIO version. WCSLIB = '5.15 ' / WCSLIB version. GNUASTRO= '0.3' / GNU Astronomy Utilities version. END  File: gnuastro.info, Node: Extensions and Tables, Next: Image manipulation, Prev: Common program behavior, Up: Top 5 Extensions and Tables *********************** This chapter documents those Gnuastro programs that don’t directly operate on the contents of the data file, they just print information, or convert from different data types. Before working on a FITS file, it is commonly the case that you are not sure how many extensions it has within it and also what each extension is (image, table or blank). In such cases, Header (see *note Header::) can be handy by printing the full header of a FITS file to the terminal for easy inspection. In other cases you want to use the data in a FITS file in other programs (for example in reports) that don’t recognize the FITS format, for example converting a FITS image into a Jpeg, or PDF format image. ConvertType (see *note ConvertType::) was built for such situations. Finally, the FITS format is not just for images, it can also store tables. Binary tables in particular can be very useful in storing very large catalogs or tables compared to a plain text file. Table (see *note Table::) can be used to choose certain table columns in a FITS table and see them as a human readable output on the terminal, or to save them in another plain text or FITS table. * Menu: * Header:: Print and manipulate data file header. * ConvertType:: Convert data to various formats. * Table:: Read and Write FITS tables to plain text.  File: gnuastro.info, Node: Header, Next: ConvertType, Prev: Extensions and Tables, Up: Extensions and Tables 5.1 Header ========== The FITS standard requires each extension of a FITS file to have a header, giving basic information about what is in that extension. Each line in the header is for one keyword, specifying its name, value and a short comment string. Besides the basic information, the headers also contain vital information about the data, how they were processed, the instrument specifications that took the image and also the World Coordinate System that is used to translate pixel coordinates to sky or spectrum coordinates on the image or table. * Menu: * Invoking astheader:: Arguments and options to Header.  File: gnuastro.info, Node: Invoking astheader, Prev: Header, Up: Header 5.1.1 Invoking Header --------------------- Header can print or manipulate the header information in an extension of an astronomical data file. The executable name is ‘astheader’ with the following general template $ astheader [OPTION...] ASTRdata One line examples: $ astheader image.fits $ astheader --update=OLDKEY,153.034,"Old keyword comment" $ astheader --remove=COMMENT --comment="Anything you like ;-)." $ astheader --write=MYKEY1,20.00,"An example keyword" --write=MYKEY2,fd If no keyword modification options are given, the full header of the given HDU will be printed on the command-line. If any of the keywords are to be modified, the headers of the input file will be changed. If you want to keep the original FITS file, it is easiest to create a copy first and then run Header on that. In the FITS standard, keywords are always uppercase. So case does not matter in the input or output keyword names you specify. Most of the options can accept multiple instances in one command. For example you can add multiple keywords to delete by calling delete multiple times, since repeated keywords are allowed, you can even delete the same keyword multiple times. The action of such options will start from the top most keyword. *FITS STANDARD KEYWORDS:* Some header keywords are necessary for later operations on a FITS file, for example BITPIX or NAXIS, see the FITS standard for their full list. If you modify (for example remove or rename) such keywords, the FITS file extension might not be usable any more. Also be careful for the world coordinate system keywords, if you modify or change their values, any future world coordinate system (like RA and Dec) measurements on the image will also change. *PRECEDENCE:* The order of operations are as follows. Note that while the order within each class of actions is preserved, the order of individual actions is not. So irrespective of what order you called ‘--delete’ and ‘--update’. First all the delete operations are going to take effect then the update operations. 1. ‘--delete’ 2. ‘--rename’ 3. ‘--update’ 4. ‘--write’ 5. ‘--asis’ 6. ‘--history’ 7. ‘--comment’ 8. ‘--date’ All possible syntax errors will be reported before the keywords are actually written. FITS errors during any of these actions will be reported, but Header won’t stop until all the operations are complete. If ‘quitonerror’ is called, then Header will immediately stop upon the first error. If only a certain set of header keywords are desired, it is easiest to pipe the output of Header to GNU Grep. Grep is a very powerful and advanced tool to search strings which is precisely made for such situations. For example if you only want to check the size of an image FITS HDU, you can run: $ astheader input.fits | grep NAXIS The options particular to Header can be seen below. See *note Common options:: for a list of the options that are common to all Gnuastro programs, they are not repeated here. ‘-a’ ‘--asis’ (‘=STR’) Write the string within this argument exactly into the FITS file header with no modifications. If it does not conform to the FITS standards, then it might cause trouble, so please be very careful with this option. If you want to define the keyword from scratch, it is best to use the ‘--write’ option (see below) and let CFITSIO worry about the standards. The best way to use this option is when you want to add a keyword from one FITS file to another unchanged and untouched. Below is an example of such a case that can be very useful sometimes: $ key=$(astheader firstimage.fits | grep KEYWORD) $ astheader --asis="$key" secondimage.fits In particular note the double quotation signs (<">) around the reference to the ‘key’ shell variable (‘$key’), since FITS keywords usually have lots of space characters, if this variable is not enclosed within double quotation marks, the shell will only give the first word in the full keyword to this option, which will definitely be a non-standard FITS keyword and will make it hard to work on the file afterwords. See the “Quoting†section of the GNU Bash manual for more information if your keyword has the special characters <$>, <`>, or <\>. ‘-d’ ‘--delete’ (‘=STR’) Delete one instance of the desired keyword. Multiple instances of ‘--delete’ can be given (possibly even for the same keyword). All keywords given will be removed from the headers in the opposite order (last given keyword will be deleted first). If the keyword doesn’t exist, Header will give a warning and return with a non-zero value, but will not stop. ‘-r’ ‘--rename’ (‘=STR’) Rename a keyword to a new value. The old name and the new name should be separated by either a comma (<,>) or a space character. Note that if you use a space character, you have to put the value to this option within double quotation marks (<">) so the space character is not interpreted as an option separator. Multiple instances of ‘--rename’ can be given in one command. The keywords will be renamed in the specified order. ‘-u’ ‘--update’ (‘=STR’) Update a keyword, its value, its comments and its units all defined separately. If there are multiple instances of the keyword in the header, they will be changed from top to bottom (with multiple ‘--update’ options). The format of the values to this option can best be specified with an example: --update=KEYWORD,value,"comments for this keyword",unit The value can be any numerical or string value(1). Other than the ‘KEYWORD’, all the other values are optional. To leave a given token empty, follow the preceding comma (<,>) immediately with the next. If any space character is present around the commas, it will be considered part of the respective token. So if more than one token has space characters within it, the safest method to specify a value to this option is to put double quotation marks around each individual token that needs it. Note that without double quotation marks, space characters will be seen as option separators and can lead to undefined behavior. ‘-w’ ‘--write’ (‘=STR’) Write a keyword to the header. For the possible value input formats, comments and units for the keyword, see the ‘--update’ option above. ‘-H’ ‘--history’ (‘=STR’) Add a ‘HISTORY’ keyword to the header. The string given to this keyword will be separated into multiple keyword cards if it is longer than 70 characters. With each run only one value for the ‘--history’ option will be read. If there are multiple, it is the last one. ‘-c’ ‘--comment’ (‘=STR’) Add a ‘COMMENT’ keyword to the header. Similar to the explanation for ‘--history’ above. ‘-t’ ‘--date’ Put the current date and time in the header. If the ‘DATE’ keyword already exists in the header, it will be updated. ‘-Q’ ‘--quitonerror’ Quit if any of the operations above are not successful. By default if an error occurs, Header will warn the user of the faulty keyword and continue with the rest of actions. ---------- Footnotes ---------- (1) Some tricky situations arise with values like ‘‘87095e5’’, if this was intended to be a number it will be kept in the header as ‘8709500000’ and there is no problem. But this can also be a shortened Git commit hash. In the latter case, it should be treated as a string and stored as it is written. Commit hashes are very important in keeping the history of a file during your research and such values might arise without you noticing them in your reproduction pipeline. One solution is to use ‘git describe’ instead of the short hash alone. A less recommended solution is to add a space after the commit hash and Header will write the value as ‘‘87095e5 ’’ in the header. If you later compare the strings on the shell, the space character will be ignored by the shell in the latter solution and there will be no problem.  File: gnuastro.info, Node: ConvertType, Next: Table, Prev: Header, Up: Extensions and Tables 5.2 ConvertType =============== The formats of astronomical data were defined mainly for archiving and processing. In other situations, the data might be useful in other formats. For example, when you are writing a paper or report or if you are making slides for a talk, you can’t use a FITS image. Other image formats should be used. In other cases you might want your pixel values in a table format as plain text for input to other programs that don’t recognize FITS, or to include as a table in your report. ConvertType is created for such situations. The various types will increase with future updates and based on need. The conversion is not only one way (from FITS to other formats), but two ways (except the EPS and PDF formats). So you can convert a JPEG image or text file into a FITS image. Basically, other than EPS, you can use any of the recognized formats as different color channel inputs to get any of the recognized outputs. So before explaining the options and arguments, first a short description of the recognized files types will be given followed a short introduction to digital color. * Menu: * Recognized file types:: Recognized file types * Color:: Some explanations on color. * Invoking astconvertt:: Options and arguments to ConvertType.  File: gnuastro.info, Node: Recognized file types, Next: Color, Prev: ConvertType, Up: ConvertType 5.2.1 Recognized file types --------------------------- The various standards and the file name extensions recognized by ConvertType are listed below. FITS or IMH Astronomical data are commonly stored in the FITS format (and in older data sets in IRAF ‘.imh’ format), a list of file name suffixes which indicate that the file is in this format is given in *note Arguments::. Each extension of a FITS image only has one value per pixel, so when used as input, each input FITS image contributes as one color channel. If you want multiple extensions in one FITS file for different color channels, you have to repeat the file name multiple times and use the ‘--hdu’, ‘--hdu2’, ‘--hdu3’ or ‘--hdu4’ options to specify the different extensions. JPEG The JPEG standard was created by the Joint photographic experts group. It is currently one of the most commonly used image formats. Its major advantage is the compression algorithm that is defined by the standard. Like the FITS standard, this is a raster graphics format, which means that it is pixelated. A JPEG file can have 1 (for grayscale), 3 (for RGB) and 4 (for CMYK) color channels. If you only want to convert one JPEG image into other formats, there is no problem, however, if you want to use it in combination with other input files, make sure that the final number of color channels does not exceed four. If it does, then ConvertType will abort and notify you. The file name endings that are recognized as a JPEG file for input are: ‘.jpg’, ‘.JPG’, ‘.jpeg’, ‘.JPEG’, ‘.jpe’, ‘.jif’, ‘.jfif’ and ‘.jfi’. EPS The Encapsulated PostScript (EPS) format is essentially a one page PostScript file which has a specified size. PostScript also includes non-image data, for example lines and texts. It is a fully functional programming language to describe a document. Therefore in ConvertType, EPS is only an output format and cannot be used as input. Contrary to the FITS or JPEG formats, PostScript is not a raster format, but is categorized as vector graphics. The Portable Document Format (PDF) is currently the most common format for documents. Some believe that PDF has replaced PostScript and that PostScript is now obsolete. This view is wrong, a PostScript file is an actual plain text file that can be edited like any program source with any text editor. To be able to display its programmed content or print, it needs to pass through a processor or compiler. A PDF file can be thought of as the processed output of the compiler on an input PostScript file. PostScript, EPS and PDF were created and are registered by Adobe Systems. With these features in mind, you can see that when you are compiling a document with TeX or LaTeX, using an EPS file is much more low level than a JPEG and thus you have much greater control and therefore quality. Since it also includes vector graphic lines we also use such lines to make a thin border around the image to make its appearance in the document much better. No matter the resolution of the display or printer, these lines will always be clear and not pixelated. In the future, addition of text might be included (for example labels or object IDs) on the EPS output. However, this can be done better with tools within TeX or LaTeX such as PGF/Tikz(1). If the final input image (possibly after all operations on the flux explained below) is a binary image or only has two colors of black and white (in segmentation maps for example), then PostScript has another great advantage compared to other formats. It allows for 1 bit pixels (pixels with a value of 0 or 1), this can decrease the output file size by 8 times. So if a grayscale image is binary, ConvertType will exploit this property in the EPS and PDF (see below) outputs. The standard formats for an EPS file are ‘.eps’, ‘.EPS’, ‘.epsf’ and ‘.epsi’. The EPS outputs of ConvertType have the ‘.eps’ suffix. PDF As explained above, a PDF document is a static document description format, viewing its result is therefore much faster and more efficient than PostScript. To create a PDF output, ConvertType will make a PostScript page description and convert that to PDF using GPL Ghostscript. The suffixes recognized for a PDF file are: ‘.pdf’, ‘.PDF’. If GPL Ghostscript cannot be run on the PostScript file, it will remain and a warning will be printed. ‘blank’ This is not actually a file type! But can be used to fill one color channel with a blank value. If this argument is given for any color channel, that channel will not be used in the output. Plain text Plain text files have the advantage that they can be viewed with any text editor or on the command-line. Most programs also support input as plain text files. In ConvertType, if the input arguments do not have any of the extensions listed above for other formats, the input is assumed to be a text file. Each plain text file is considered to contain one color channel. There is no standard output for plain text files. If any of the extension above is mis-spelled, this will result in the output becoming a plain text file with that (short) name. If this happens, ConvertType will warn you and write the output as a plain text file. If you don’t want that warning, set your plain text output file names longer than 5 characters. When converting an image to plain text, consider the fact that if the image is large the number of columns in each line will become very large, possibly making it very hard to open in some text editors. ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: Color, Next: Invoking astconvertt, Prev: Recognized file types, Up: ConvertType 5.2.2 Color ----------- An image is a two dimensional array of 2 dimensional elements called pixels. If each pixel only has one value, the image is known as a grayscale image and no color is defined. The range of values in the image can be interpreted as shades of any color, it is customary to use shades of black or grayscale. However, to produce the color spectrum in the digital world, several primary colors must be mixed. Therefore in a color image, each pixel has several values depending on how many primary colors were chosen. For example on the digital monitor or color digital cameras, all colors are built by mixing the three colors of Red-Green-Blue (RGB) with various proportions. However, for printing on paper, standard printers use the Cyan-Magenta-Yellow-Key (CMYK, Key=black) color space. Therefore when printing an RGB image, usually a transformation of color spaces will be necessary. In a colored digital camera, a color image is produced by dividing the pixel’s area between three colors (filters). However in astronomy due to the intrinsic faintness of most of the targets, the collecting area of the pixel is very important for us. Hence the full area of the pixel is used and one value is stored for that pixel in the end. One color filter is used for the whole image. Thus a FITS image is inherently a grayscale image and no color can be defined for it. One way to represent a grayscale image in different color spaces is to use the same proportions of the primary colors in each pixel. This is the common way most FITS image converters work: they fill all the channels with the same values. The downside is two fold: • Three (for RGB) or four (for CMYK) values have to be stored for every pixel, this makes the output file very heavy (in terms of bytes). • If printing, the printing errors of each color channel can make the printed image slightly more blurred than it actually is. To solve both these problems, the best way is to save the FITS image into the black channel of the CMYK color space. In the RGB color space all three channels have to be used. The JPEG standard is the only common standard that accepts CMYK color space, that is why currently only the JPEG standard is included and not the PNG standard for example. The JPEG and EPS standards set two sizes for the number of bits in each channel: 8-bit and 12-bit. The former is by far the most common and is what is used in ConvertType. Therefore, each channel should have values between 0 to 2^8-1=255. From this we see how each pixel in a grayscale image is one byte (8 bits) long, in an RGB image, it is 3bytes long and in CMYK it is 4bytes long. But thanks to the JPEG compression algorithms, when all the pixels of one channel have the same value, that channel is compressed to one pixel. Therefore a Grayscale image and a CMYK image that has only the K-channel filled are approximately the same file size.  File: gnuastro.info, Node: Invoking astconvertt, Prev: Color, Up: ConvertType 5.2.3 Invoking ConvertType -------------------------- ConvertType will convert any recognized input file type to any specified output type. The executable name is ‘astconvertt’ with the following general template $ astconvertt [OPTION...] InputFile [InputFile2] ... [InputFile4] One line examples: $ astconvertt M31.fits --output=pdf $ astconvertt galaxy.jpg -ogalaxy.fits $ astconvertt f1.txt f2.txt f3.fits -o.jpg $ astconvertt M31_r.fits M31_g.fits blank -oeps The file type of the output will be specified with the (possibly complete) file name given to the ‘--output’ option, which can either be given on the command-line or in any of the configuration files (see *note Configuration files::). Note that if the output suffix is not recognized, it will default to plain text format, see *note Recognized file types::. The order of multiple input files is important. After reading the input file(s) the number of color channels in all the inputs will be used to define which color space is being used for the outputs and how each color channel is interpreted. Note that one file might have more than one color channel (for example in the JPEG format). If there is one color channel the output is grayscale, if three input color channels are given they are respectively considered to be the red, green and blue color channels and if there are four color channels they are respectively considered to be cyan, magenta, yellow and black. The value to ‘--output’ (or ‘-o’) can be either a full file name or just the suffix of the desired output format. In the former case, that same name will be used for the output. In the latter case, the name of the output file will be set based on the automatic output guidelines, see *note Automatic output::. Note that the suffix name can optionally start a ‘.’ (dot), so for example ‘--output=.jpg’ and ‘--output=jpg’ are equivalent. Be careful that if you want your output in plain text, you have to give the full file name. So if ‘-otxt’ or ‘--output=.txt’ are given, the output file will be named ‘txt’ or ‘.txt’ (the latter will be a hidden file!). Besides the common set of options explained in *note Common options::, the options to ConvertType can be classified into input, output and flux related options. The majority of the options are to do with the flux range. Astronomical data usually have a very large dynamic range (difference between maximum and minimum value) and different subjects might be better demonstrated with a limited flux range. Input: ‘--hdu2’ If the second input file is a FITS file, the value to this option will be used to specify which HDU will be used. Note that for the first file, the (‘--hdu’ or ‘-h’ in the common options is used) ‘--hdu3’ The HDU of the third input FITS file. ‘--hdu4’ The HDU of the fourth input FITS file. Output: ‘-w’ ‘--widthincm’ (‘=FLT’) The width of the output in centimeters. This is only relevant for those formats that accept such a width (not plain text for example). For most digital purposes, the number of pixels is far more important than the value to this parameter because you can adjust the absolute width (in inches or centimeters) in your document preparation program. ‘-b’ ‘--borderwidth’ (‘=INT’) The width of the border to be put around the EPS and PDF outputs in units of PostScript points. There are 72 or 28.35 PostScript points in an inch or centimeter respectively. In other words, there are roughly 3 PostScript points in every millimeter. If you are planning on adding a border, its significance is highly correlated with the value you give to the ‘--widthincm’ parameter. Unfortunately in the document structuring convention of the PostScript language, the “bounding box†has to be in units of PostScript points with no fractions allowed. So the border values only have to be specified in integers. To have a final border that is thinner than one PostScript point in your document, you can ask for a larger width in ConvertType and then scale down the output EPS or PDF file in your document preparation program. For example by setting ‘width’ in your ‘includegraphics’ command in TeX or LaTeX. Since it is vector graphics, the changes of size have no effect on the quality of your output quality (pixels don’t get different values). ‘-x’ ‘--hex’ Use Hexadecimal encoding in creating EPS output. By default the ASCII85 encoding is used which provides a much better compression ratio. When converted to PDF (or included in TeX or LaTeX which is finally saved as a PDF file), an efficient binary encoding is used which is far more efficient than both of them. The choice of EPS encoding will thus have no effect on the final PDF. So if you want to transfer your EPS files (for example if you want to submit your paper to arXiv or journals in PostScript), their storage might become important if you have large images or lots of small ones. By default ASCII85 encoding is used which offers a much better compression ratio (nearly 40 percent) compared to Hexadecimal encoding. ‘-u’ ‘--quality’ (‘=INT’) The quality (compression) of the output JPEG file with values from 0 to 100 (inclusive). For other formats the value to this option is ignored. Note that only in grayscale (when one input color channel is given) will this actually be the exact quality (each pixel will correspond to one input value). If it is in color mode, some degradation will occur. While the JPEG standard does support loss-less graphics, it is not commonly supported. Flux range: ‘-c’ ‘--change’ (‘=STR’) Change pixel values with the following format ‘"from1:to1, from2:to2,..."’. This option is very useful in displaying labeled pixels (not actual data images which have noise) like segmentation maps. In labeled images, usually a group of pixels have a fixed integer value. With this option, you can manipulate the labels before the image is displayed to get a better output for print or to emphasize on a particular set of labels and ignore the rest. The labels in the images will be changed in the same order given. By default first the pixel values will be converted then the pixel values will be truncated (see ‘--fluxlow’ and ‘--fluxhigh’). You can use any number for the values irrespective of your final output, your given values are stored and used in the double precision floating point format. So for example if your input image has labels from 1 to 20000 and you only want to display those with labels 957 and 11342 then you can run ConvertType with these options: $ astconvertt --change=957:50000,11342:50001 --fluxlow=5e4 \ --fluxhigh=1e5 segmentationmap.fits --output=jpg While the output JPEG format is only 8 bit, this operation is done in an intermediate step which is stored in double precision floating point. The pixel values are converted to 8-bit after all operations on the input fluxes have been complete. By placing the value in double quotes you can use as many spaces as you like for better readability. ‘-C’ ‘--changeaftertrunc’ Change pixel values (with ‘--change’) after truncation of the flux values, by default it is the opposite. ‘-L’ ‘--fluxlow’ (‘=FLT’) The minimum flux (pixel value) to display in the output image, any pixel value below this value will be set to this value in the output. If the value to this option is the same as ‘--fluxmax’, then no flux truncation will be applied. Note that when multiple channels are given, this value is used for all the color channels. ‘-H’ ‘--fluxhigh’ (‘=FLT’) The maximum flux (pixel value) to display in the output image, see ‘--fluxlow’. ‘-m’ ‘--maxbyte’ (‘=INT’) This is only used for the JPEG and EPS output formats which have an 8-bit space for each channel of each pixel. The maximum value in each pixel can therefore be $2^8-1=255$. With this option you can change (decrease) the maximum value. By doing so you will decrease the dynamic range. It can be useful if you plan to use those values for other purposes. ‘-i’ ‘--flminbyte’ (‘=INT’) If the lowest pixel value in the input channels is larger than the value to ‘--fluxlow’, then that input value will be redundant. In some situations it might be necessary to set the minimum byte value (0) to correspond to that flux even if the data do not reach that value. With this option you can do this. Note that if the minimum pixel value is smaller than ‘--fluxlow’, then this option is redundant. ‘-a’ ‘--fhmaxbyte’ (‘=INT’) See ‘--flminbyte’. ‘-l’ ‘--log’ Display the logarithm of the input data. This is done after the conversion and flux truncation steps, see above. ‘-n’ ‘--noinvert’ For 8-bit output types (JPEG and EPS for example) the final value that is stored is inverted so white becomes black and vice versa. The reason for this is that astronomical images usually have a very large area of blank sky in them. The result will be that a large are of the image will be black. Therefore, by default the 8-bit values are inverted so the images blend in better with the text in a document. Note that this behaviour is ideal for grayscale images, if you want a color image, the colors are going to be mixed up. For color images it is best to call this option so the image is not inverted.  File: gnuastro.info, Node: Table, Prev: ConvertType, Up: Extensions and Tables 5.3 Table ========= The FITS standard is not just for storing astronomical images, from its early days, it also included tables. Tables are the products of processing astronomical images and spectra. For example in Gnuastro, MakeCatalog will process the defined pixels over an object and produce a catalog (see *note MakeCatalog::). For each identified object, MakeCatalog can print its position on the image or sky, its total brightness and many other information that is deducible from the given image. Each one of these properties is a column in its output catalog (or table) and for each input object, we have a row. When there are only a small number of objects (rows) and not too many properties (columns), then a simple plain text file is mainly enough to store, transfer, or even use the produced data. However, to be more efficient in all these aspects, astronomers have defined the FITS binary table standard to store data in a binary (0 and 1) format, not plain text. This can offer major advantages in all those aspects: the file size will be greatly reduced and the reading and writing will be faster (because the RAM and CPU also work in binary). The FITS standard also defines a standard for ASCII tables, where the data are stored in the human readable ASCII format, but within the FITS file structure. These are mainly useful for keeping ASCII data along with images and possibly binary data as multiple (conceptually related) extensions within a FITS file. However, this comes at a cost: binary tables are not easily readable by human eyes. There is no standard on how the zero and ones should be interpretted. The Unix-like operating systems have flourished because of a simple fact: communication between the various tools is based on human readable characters(1). So while the FITS table standards are very beneficial for the tools that recognize them, they are hard to use in the vast majority of available software. This creates limitations for their generic use. ‘Table’ is Gnuastro’s solution to this problem. With Table, FITS tables (ASCII or binary) are directly accessible to the Unix-like operating systems power-users (those working the command-line or shell, see *note Command-line interface::). With Table, a FITS table (in binary or ASCII formats) is only one command away from AWK (or any other tool you want to use). Just like a plain text file that you read with the ‘cat’ command. You can pipe the output of Table into any other tool for higher-level processing, see the examples in *note Invoking asttable:: for some very simple examples. * Menu: * Invoking asttable:: Options and arguments to Table. ---------- Footnotes ---------- (1) In “The art of Unix programmingâ€, Eric Raymond makes this suggestion to programmers: “When you feel the urge to design a complex binary file format, or a complex binary application protocol, it is generally wise to lie down until the feeling passes.â€. This is a great book and strongly recommended, give it a look if you want to truly enjoy your work/life in this environment.  File: gnuastro.info, Node: Invoking asttable, Prev: Table, Up: Table 5.3.1 Invoking Table -------------------- Table will convert FITS binary and ASCII tables into other such tables, or print them on the command-line, or save them in a plain text file. Output columns can also be determined by number or regular expression matching of column names. The executable name is ‘asttable’ with the following general template $ asttable [OPTION...] InputFile One line examples: ## Get the table column information (name, data type, or units) $ asttable bintab.fits --information ## Only print those columns which have a name starting with "MAG_" $ asttable bintab.fits --columns=^MAG_ ## Only print the 2nd column, and the third column multiplied by 5 $ asttable bintab.fits | awk '{print $2, 5*$3}' ## Only print those rows with a value in the 10th column above 100000 $ asttable bintab.fits | awk '$10>10e5 {print}' ## Sort the output columns by the third column, save output $ asttable bintab.fits | sort -k3 > output.txt ## Convert a plain text table to a binary FITS table $ asttable plaintext.txt --output=inbinary.fits Table can accept plain text files, or binary and ASCII FITS table extensions in a FITS file. For the full list of options common to all Gnuastro utilities please see *note Common options::. Options can also be stored in directory, user or system-wide configuration files to avoid repeating on the command-line, see *note Configuration files::. Currently all plain text files are processed (and thus printed, or saved to a binary FITS table) as double floating point types. We are still working on this many many more features. Table does not follow Automatic output that is common in most Gnuastro, see *note Automatic output::. If no value is given to the ‘--output’ option, the desired columns will be printed to the standard output (on the command-line). This feature makes it very useful to directly pipe the output as input to other programs as the examples above demonstrate. Note that the options below which relate to print formatting are only relevant when the output is in human readable format (on the command-line and plain text files), they are ignored when the output is a binary FITS table. ‘-i’ ‘--information’ Print the information for each column and abort. The information for each column will be printed as a row on the command-line. The column name (if present), units (if present) and datatype will printed. Note that the FITS standard does not require a name or units for columns, only the datatype is mandatory. ‘-c’ ‘--column’ (‘=STR’ or ‘=INT’) Specify the columns to output for this table. If an integer number is given, the column number will be used (counting from 1). Otherwise the value (a string) will be passed to an internal regular expression processor which will try to match all the columns in the table with the given regular expression. Currently only FITS tables might have column names (it is an optional feature in the FITS standard). There is currently no particular standard to name plain text columns. This option can be called any number of times with one run of Table. The order of the output columns will be determined by the input order. This option is also not mandatory. If not given, all the input table columns are output. Regular expressions are a very powerful tool in matching text and since FITS binary tables usually have a large number of columns, this feature can greatly simply the selection of the output columns. ‘-I’ ‘--ignorescase’ Ignore case while matching the column names with the value(s) of the ‘--column’ option. The FITS standard suggests to treat the column names as case insensitive, however it is not a requirement. ‘--feg’ (‘=STR’) Format of printing floating point numbers in non-binary outputs. It can only accept one of the three following values (same as C’s ‘printf’): • : Print complete floating point value, this is good when the numbers aren’t too small, for example $3.286$. But it will print all the zeros in $3.2\times10^{-15}$. • : Only print in exponential format. This is good for very large or very small numbers, but can make reading the values of more ordinary numbers a little hard. • : Let the system choose which representation is better for the number. ‘--sintwidth’ (‘=INT’) The minimum width (number of characters) for printing columns of shorter integer datatypes. The shorter datatypes are considered to be signed and unsigned characters, short integers, integers. ‘--lintwidth’ (‘=INT’) The minimum width (number of characters) for printing columns of longer datatypes. The longer datatypes are considered to be ‘long’ and ‘longlong’ types. ‘--floatwidth’ (‘=INT’) The minimum width (number of characters) for printing columns of single precision floating point datatypes. ‘--doublewidth’ (‘=INT’) The minimum width (number of characters) for printing columns of double precision floating point datatypes. ‘--strwidth’ (‘=INT’) The minimum width (number of characters) for printing columns of strings (given as one column, the FITS standard allows ASCII strings as table elements). ‘--floatprecision’ (‘=INT’) The number of digits to print after the floating point for single precision floating point numbers. ‘--doubleprecision’ (‘=INT’) The number of digits to print after the floating point for double precision floating point numbers. ‘--fitstabletype’ (‘=STR’) The type of FITS table when a FITS file is specified as the output. This option can only have two values: ‘binary’, or ‘ascii’. However, currently ASCII FITS table outputs are not yet implemented due to lack of need. If you need it, please get in touch with so we implement it.  File: gnuastro.info, Node: Image manipulation, Next: Image analysis, Prev: Extensions and Tables, Up: Top 6 Image manipulation ******************** Images are one of the major formats of data that is used in astronomy. The functions in this chapter explain the GNU Astronomy Utilities which are provided for their manipulation. For example cropping out a part of a larger image or convolving the image with a given kernel or applying a transformation to it. * Menu: * ImageCrop:: Crop region(s) from FITS image(s). * Arithmetic:: Arithmetic on input data. * Convolve:: Convolve an image with a kernel. * ImageWarp:: Warp/Transform an image to a different grid. * SubtractSky:: Find the sky and subtract it from image.  File: gnuastro.info, Node: ImageCrop, Next: Arithmetic, Prev: Image manipulation, Up: Image manipulation 6.1 ImageCrop ============= Astronomical images are often very large, filled with thousands of galaxies. It often happens that you only want a section of the image, or you have a catalog of sources and you want to visually analyze them in small postage stamps. ImageCrop is made to do all these things. When more than one crop is required, ImageCrop will divide the crops between multiple threads to significantly reduce the run time. Astronomical surveys are usually extremely large. So large in fact, that the whole survey will not fit into a reasonably sized file. Because of this surveys usually cut the final image into separate tiles and store each tile in a file. For example the COSMOS survey’s Hubble space telescope, ACS F814W image consists of 81 separate FITS images, with each one having a volume of 1.7 Giga bytes. Even though the tile sizes are chosen to be large enough that too many galaxies don’t fall on the edges of the tiles, inevitably some do and if you simply crop the image of the galaxy from that one tile, you will miss a large area of the surrounding sky (which is essential in estimating the noise). Therefore in its WCS mode, ImageCrop will stitch parts of the tiles that are relevant for a target (with the given width) from all the input images that cover that region into the output. Of course, the tiles have to be present in the list of input files. ImageCrop also has facilities to crop arbitrary polygons from a set of tiles by stitching the relevant parts of different tiles within the polygon, see ‘--polygon’ in *note Invoking astimgcrop::. Alternatively, it can crop out rectangular regions from one image which can come in handy when removing the bias pixels in raw image processing, see *note Crop section syntax::. * Menu: * ImageCrop modes:: Basic ImageCrop modes. * Crop section syntax:: How to define a section to crop. * Blank pixels:: Pixels with no value. * Invoking astimgcrop:: Calling ImageCrop on the command-line  File: gnuastro.info, Node: ImageCrop modes, Next: Crop section syntax, Prev: ImageCrop, Up: ImageCrop 6.1.1 ImageCrop modes --------------------- In order to be as comprehensive as possible, ImageCrop has two major modes of operation listed below. Image The image mode uses the pixel coordinates. Depending on your command line options, this mode consists of three sub-modes. In image mode, only one image may be input. • Catalog (multiple crops). Coordinates are read from a text file. The ‘--xcol’ and ‘--ycol’ columns in the catalog are interpreted as the center of a square crop box whose width is specified with the ‘--iwidth’ option in pixels. Since the given pixel has to be on the center, the width has to be an odd number, so if you give an even number for the width, it will be added by one. If a catalog file name is provided (with ‘--imagemode’ activated of course) this mode will be used. • Center (one crop). The box center is given on the command-line with the ‘--xc’ and ‘--yc’ parameters. The image width is similar to above. • Section (one crop). You can specify the section of pixels along each axis in the image which you want to be cropped with the ‘--section’ option. See *note Crop section syntax:: for a full explanation on the syntax of specifying the desired region. The latter two cases will only have one crop box. In both cases, ImageCrop will go into the image mode, irrespective of calling ‘--wcsmode’ or the default mode. In the first two cases, since you specify a central pixel, the crop box will be a square with an odd number of pixels on the side, so your desired pixel sits right in the center, see *note Blank pixels:: on how to disable this for cases when the box exceeds the image size. WCS The Right ascension (RA) and Declination (Dec) of the objects in a catalog is used to define the central position of each postage stamp. In this mode, the width (‘--wwidth’) is read in units of arc seconds and multiple images (tiles in a survey) can be input. If the objects are closer to the edge of the image than half the required width, other tiles (if they are present in the input files) are used to fill the empty space. The square output cropped box will have an odd number of pixels on the side. In this mode, the input images do not necessarily have to be the same size, each individual tile can even be smaller than the final crop. In any case, any part of any of the input images which overlaps with the desired region will be used in the crop. Note that if there is an over lap, the pixels from the last input image read are going to be used. The input images all just have to be aligned with the celestial coordinates, see the caution note below. Similar to the image mode, there are two sub-modes: • Catalog (multiple crops). Similar to catalog mode in image mode. The RA and Dec column should be specified in the catalog (‘--racol’ and ‘--deccol’). • Center (one crop). You can specify the center of only one crop box (no matter how many input images there are) with the options ‘--ra’ and ‘--dec’. If it exists in the input images, it will be cropped similar to the catalog mode. If automatic output is triggered (you don’t specify a file name for ‘--output’) and several of the input images are used to stitch and crop the region around the central point, the name of the first input will be used in automatic output, see *note Automatic output::. *CAUTION:* In WCS mode, the image has to be aligned with the celestial coordinates, such that the first FITS axis is parallel (opposite direction) to the Right Ascension (RA) while the second FITS axis is parallel to the declination. If these conditions aren’t met for an image, ImageCrop will warn you and abort. You have to use other tools to transform the image to the correct directions. In short, if you don’t specify a catalog, you have to specify box coordinates manually on the command-line. When you do specify a catalog, ImageCrop has to be in one of the two major modes (‘--imgmode’ or ‘--wcsmode’). Note that the single crop box parameters specified in the sub-modes will not be written to or read from the configuration file, they have to be specified on each execution.  File: gnuastro.info, Node: Crop section syntax, Next: Blank pixels, Prev: ImageCrop modes, Up: ImageCrop 6.1.2 Crop section syntax ------------------------- When in image mode, one of the methods to crop only one rectangular section from the input image is to use the ‘--section’ option. ImageCrop has a powerful syntax to read the box parameters from a string of characters. If you leave certain parts of the string to be empty, ImageCrop can fill them for you based on the input image sizes. To define a box, you need the coordinates of two points: the first pixel in the box at (‘X1’, ‘Y1’) and the pixel which is immediately outside of the box (‘X2, Y2’), four coordinates in total. The four coordinates can be specified with one string in this format: ‘X1:X2,Y1:Y2’. It is given to the ‘--section’ option. Therefore, the pixels along the first axis that are \geq‘X1’ and <‘X2’ will be included in the cropped image. The same goes for the second axis. Note that each different term will be read as an integer, not a float (there are no sub-pixels in ImageCrop, you can use ImageWarp to shift the matrix with any sub-pixel distance, then crop the warped image, see *note ImageWarp::). Also, following the FITS standard, pixel indexes along each axis start from unity(1) not zero(0). You can omit any of the values and they will be filled automatically. The left hand side of the colon (‘:’) will be filled with ‘1’, and the right side with the image size. So, ‘2:,:’ will include the full range of pixels along the second axis and only those with a first axis index larger than ‘2’ in the first axis. If the colon is omitted for a dimension, then the full range is automatically used. So the same string is also equal to ‘2:,’ or ‘2:’ or even ‘2’. If you want such a case for the second axis, you should set it to: ‘,2’. If you specify a negative value, it will be seen as before the indexes of the image which are outside the image along the bottom or left sides when viewed in SAO ds9. In case you want to count from the top or right sides of the image, you can use an asterisk (‘*’). When confronted with a ‘*’, ImageCrop will replace it with the maximum length of the image in that dimension. So ‘*-10:*+10,*-20:*+20’ will mean that the crop box will be 20\times40 pixels in size and only include the top corner of the input image with 3/4 of the image being covered by blank pixels, see *note Blank pixels::. If you feel more comfortable with space characters between the values, you can use as many space characters as you wish, just be careful to put your value in double quotes, for example ‘--section="5:200, 123:854"’. If you forget, anything after the first space will not be seen by ‘--section’, because the unquoted space character is one of the characters that separates options on the command-line.  File: gnuastro.info, Node: Blank pixels, Next: Invoking astimgcrop, Prev: Crop section syntax, Up: ImageCrop 6.1.3 Blank pixels ------------------ The cropped box can potentially include pixels that are beyond the image range. For example when a target in the input catalog was very near the edge of the input image. The parts of the cropped image that were not in the input image will be filled with the following two values depending on the data type of the image. In both cases, SAO ds9 will not color code those pixels. • If the data type of the image is a floating point type (float or double), IEEE NaN (Not a number) will be used. • For integer types, pixels out of the image will be filled with the value of the ‘BLANK’ keyword in the cropped image header. The value assigned to it is the lowest value possible for that type, so you will probably never need it any way. Only for the unsigned character type (‘BITPIX=8’ in the FITS header), the maximum value is used because it is unsigned, the smallest value is zero which is often meaningful. You can ask for such blank regions to not be included in the output crop image using the ‘--noblank’ option. In such cases, there is no guarantee that the image size of your outputs are what you asked for. In some survey images, unfortunately they do not use the ‘BLANK’ FITS keyword. Instead they just give all pixels outside of the survey area a value of zero. So by default, when dealing with float or double image types, any values that are 0.0 are also regarded as blank regions. This can be turned off with the ‘--zeroisnotblank’ option.  File: gnuastro.info, Node: Invoking astimgcrop, Prev: Blank pixels, Up: ImageCrop 6.1.4 Invoking ImageCrop ------------------------ ImageCrop will crop a region from an image. If in WCS mode, it will also stitch parts from separate images in the input files. The executable name is ‘astimgcrop’ with the following general template $ astimgcrop [OPTION...] [ASCIIcatalog] ASTRdata ... One line examples: $ astimgcrop -I catalog.txt image.fits $ astimgcrop -W catalog.txt /mnt/data/COSMOS/*_drz.fits $ astimgcrop --section=10:*-10,10:*-10 --hdu=2 image.fits $ astimgcrop --ra=189.16704 --dec=62.218203 goodsnorth.fits $ astimgcrop --xc=568.342 --yc=2091.719 --iwidth=200 image.fits ImageCrop has one mandatory argument which is the input image name(s), shown above with ‘ASTRdata ...’. You can use shell expansions, for example ‘*’ for this if you have lots of images in WCS mode. If the crop box centers are in a catalog, you also have to provide the catalog name as an argument. Alternatively, you have to provide the crop box parameters with command-line options. When in catalog mode, ImageCrop will run in parallel unless you set ‘--numthreads=1’, see *note Threads in Gnuastro::. Note that when multiple threads are being used, in verbose mode, the outputs will not be in order. This is because the threads are asynchronous and thus not started in order. This has no effect on the output, see *note Hubble visually checks and classifies his catalog:: for a tutorial on effectively using this feature. * Menu: * astimgcrop options:: A list of all the options with explanation. * astimgcrop output:: The outputs of ImageCrop.  File: gnuastro.info, Node: astimgcrop options, Next: astimgcrop output, Prev: Invoking astimgcrop, Up: Invoking astimgcrop 6.1.4.1 ImageCrop options ......................... The options can be classified into the following contexts: Input, Output and operating mode options. Options that are common to all Gnuastro program are listed in *note Common options:: and will not be repeated here. *NOTE:* The coordinates are in the FITS format. So the first axis is the horizontal axis when viewed in SAO ds9 and the second axis is the vertical. Also in the FITS standard, counting begins from 1 (one) not 0 (zero). Input image parameters: ‘--hstartwcs’ (‘=INT’) Specify the first keyword card (line number) to start finding the input image world coordinate system information. Distortions were only recently included in WCSLIB (from version 5). Therefore until now, different telescope would apply their own specific set of WCS keywords and put them into the image header along with those that WCSLIB does recognize. So now that WCSLIB recognizes most of the standard distortion parameters, they will get confused with the old ones and give completely wrong results. For example in the CANDELS-GOODS South images(1). The two ‘--hstartwcs’ and ‘--hendwcs’ are thus provided so when using older datasets, you can specify what region in the FITS headers you want to use to read the WCS keywords. Note that this is only relevant for reading the WCS information, basic data information like the image size are read separately. These two options will only be considered when the value to ‘--hendwcs’ is larger than that of ‘--hstartwcs’. So if they are equal or ‘--hstartwcs’ is larger than ‘--hendwcs’, then all the input keywords will be parsed to get the WCS information of the image. ‘--hendwcs’ (‘=INT’) Specify the last keyword card to read for specifying the image world coordinate system on the input images. See ‘--hstartwcs’ Crop box parameters: ‘-x’ ‘--xc’ (‘=FLT’) The first FITS axis value of central position of the crop box in single image mode. ‘-y’ ‘--yc’ (‘=FLT’) The second FITS axis value of the central position of the crop box in single image mode. ‘-s’ ‘--section’ (‘=STR’) Section of the input image which you want to be cropped. See *note Crop section syntax:: for a complete explanation on the syntax required for this input. ‘-l’ ‘--polygon’ (‘=STR’) String of crop polygon vertices. Note that currently only convex polygons should be used. In the future we will make it work for all kinds of polygons. Convex polygons are polygons that do not have an internal angle more than 180 degrees. This option can be used both in the image and WCS modes. The rectangular region that completely encompasses the polygon will be kept and all the pixels that are outside of it will be removed. The syntax for the polygon vertices is similar to and simpler than that for ‘--section’. In short, the dimensions of each coordinate are separated by a comma (<,>) and each vertice is separated by a colon (<:>). You can define as many vertices as you like. If you would like to use space characters between the dimensions and vertices to make them more human-readable, then you have to put the value to this option in double quotation marks. For example let’s assume you want to work on the deepest part of the WFC3/IR images of Hubble Space Telescope eXtreme Deep Field (HST-XDF). According to the webpage (https://archive.stsci.edu/prepds/xdf/)(2) the deepest part is contained within the coordinates: [ (53.187414,-27.779152), (53.159507,-27.759633), (53.134517,-27.787144), (53.161906,-27.807208) ] They have provided mask images with only these pixels in the WFC3/IR images, but what if you also need to work on the same region in the full resolution ACS images? Also what if you want to use the CANDELS data for the shallow region? Running ImageCrop with ‘--polygon’ will easily pull out this region of the image for you irrespective of the resolution (if you have set the operating mode to WCS mode in your nearest configuration file, there is no need for ‘--wcsmode’, you may also provide many FITS image or tiles and ImageCrop will stitch them all): $ astimgcrop --wcsmode desired-filter-image(s).fits \ --polygon="53.187414,-27.779152 : 53.159507,-27.759633 : \ 53.134517,-27.787144 : 53.161906,-27.807208" ‘--outpolygon’ Keep all the regions outside the polygon and mask the inner ones with blank pixels (see *note Blank pixels::). This is practically the inverse of the default mode of treating polygons. Note that this option only works when you have only provided one input image. If multiple images are given (in WCS mode), then the full area covered by all the images has to be shown and the polygon excluded. This can lead to a very large area if large surveys like COSMOS are used. So ImageCrop will abort and notify you. In such cases, it is best to crop out the larger region you want, then mask the smaller region with this option. ‘-r’ ‘--ra’ (‘=FLT’) The first FITS axis value of central position of the crop box in single image mode. ‘-d’ ‘--dec’ (‘=FLT’) The second FITS axis value of the central position of the crop box in single image mode. ‘-i’ ‘--xcol’ (‘=INT’) Column number of the first FITS axis position of the box center, starting from zero. In SAO ds9, the first FITS axis is the horizontal axis. ‘-j’ ‘--ycol’ (‘=INT’) Column number of the second FITS axis position of the box center, starting from zero. In SAO ds9, the second FITS axis is the vertical axis. ‘-a’ ‘--iwidth’ (‘=INT’) Width the square box to crop in image mode in units of pixels. In order for the chosen central pixel to be in the center of the cropped image, the final width has to be an odd number, therefore if the value to this option is an even number, the final crop width will be one pixel larger in each dimension. If you want an even sided crop box, use the ‘--section’ option to specify the boundaries of the box, see *note Crop section syntax::. ‘-f’ ‘--racol’ (‘=INT’) Column number of Right Ascension (RA) in the input catalog, starting from zero. ‘-g’ ‘--deccol’ (‘=INT’) Column number of declination in the input catalog, starting from zero. ‘-w’ ‘--wwidth’ (‘=FLT’) The width of the crop box in WCS mode in units of arc-seconds. Output options: ‘-c’ ‘--checkcenter’ (‘=INT’) Box size of region in the center of the image to check in units of pixels. This is only used in WCS mode. Because surveys don’t often have a clean square or rectangle shape, some of the pixels on the sides of the surveys don’t have any data and are commonly filled with zero valued pixels. If the RA and Dec of any of the targets specified in the catalog fall in such regions, that cropped image will be useless! Therefore with this option, you can specify a width of a small box (3 pixels is often good enough) around the central pixel of the cropped image. If all the pixels in this small box have the value of zero, no cropped image will be created and this object will be flagged in the final log file. ‘-p’ ‘--suffix’ (‘=STR’) The suffix (or post-fix) of the output files for when you want all the cropped images to have a special ending. One case where this might be helpful is when besides the science images, you want the weight images (or exposure maps, which are also distributed with survey images) of the cropped regions too. So in one run, you can set the input images to the science images and ‘--suffix=_s.fits’. In the next run you can set the weight images as input and ‘--suffix=_w.fits’. ‘-b’ ‘--noblank’ Pixels outside of the input image that are in the crop box will not be used. By default they are filled with blank values (depending on type), see *note Blank pixels::. ‘-z’ ‘--zeroisnotblank’ In float or double images, it is common to give the value of zero to blank pixels. If the input image type is one of these two types, such pixels will also be considered as blank. You can disable this behavior with this option, see *note Blank pixels::. Operating mode options: ‘-I’ ‘--imgmode’ Operate in Image mode as described above. This option is only useful when catalog is being provided. If coordinates are given on the command-line, the mode is automatically set based on them. ‘-W’ ‘--wcsmode’ Operate in WCS mode. See explanations for ‘--imgmode’. ---------- Footnotes ---------- (1) (2)  File: gnuastro.info, Node: astimgcrop output, Prev: astimgcrop options, Up: Invoking astimgcrop 6.1.4.2 ImageCrop output ........................ When a catalog is given, the value of ‘--output’ (see *note Common options::) will be seen as the directory to store the output cropped images. In such cases, the outputs will consist of two parts: a variable part (the row number of each target starting from 1) along with a fixed string which you can set with the ‘--suffix’ option. Note that in catalog mode, only one image can be input. When the crop box is specified on the command-line, the value to ‘--output’ will be used as a file name. If no output is specified or if it is a directory, the output file name will follow the automatic output names of Gnuastro, see *note Automatic output:: for the input image. The header of each output cropped image will contain the names of the input image(s) it was cut from. If a name is longer than the 70 character space that the FITS standard allows for header keyword values, the name will be cut into several keywords from the nearest slash (). The keywords have the following format: ‘ICFn_m’. Where ‘n’ is the number of the image used in this crop and ‘m’ is the part of the name. Following the name is another keyword named ‘ICFnPIX’ which shows the pixel range from that input image in the same syntax as *note Crop section syntax::. Once done, a log file will be created in the current directory named ‘astimgcrop.log’. For each input row, this file will have three columns: 1. The cropped image file name for that row. 2. The number of input images that were used to create that image. 3. A ‘0’ if the central few pixels (value to the ‘--checkcenter’ option) are blank and ‘1’ otherwise. There are also comments on the top explaining basic information about the run. If the log file cannot be created (for example you don’t have write permission in the directory you are running ImageCrop in) or you have specifically asked for no log file (with the ‘--nolog’ option), then a log file will not be created (unless ‘--individual’ is called). The same columns will be printed in verbose mode on the command-line for each row.  File: gnuastro.info, Node: Arithmetic, Next: Convolve, Prev: ImageCrop, Up: Image manipulation 6.2 Arithmetic ============== It is commonly necessary to do arithmetic operations on the astronomical data. For example in the reduction of raw data it is necessary to subtract the Sky value (*note Sky value::) from each image image. Later (once the images as warped into a single grid using ImageWarp for example, see *note ImageWarp::), the images can be co-added or the output pixel grid is the average of the pixels of the individual input images. Arithmetic currently uses the reverse polish or postfix notation, see *note Reverse polish notation::, for more information on how to run Arithmetic, please see *note Invoking astarithmetic::. * Menu: * Reverse polish notation:: The current notation style for Arithmetic * Arithmetic operators:: List of operators known to Arithmetic * Invoking astarithmetic:: How to run Arithmetic: options and output  File: gnuastro.info, Node: Reverse polish notation, Next: Arithmetic operators, Prev: Arithmetic, Up: Arithmetic 6.2.1 Reverse polish notation ----------------------------- The most common notation for arithmetic operations is the infix notation(1) where the operator goes between the two operands, for example $4+5$. While the infix notation is the preferred way in most programming languages, currently Arithmetic does not use it since it will require parenthesis which can complicate the implementation of the code. In the near future we do plan to adopt this notation(2), but for the time being (due to time constraints on the developers), Arithmetic uses the postfix or reverse polish notation(3). The referenced Wikipedia article provides some excellent explanation on this notation but here we will give a short summary for self-sufficiency. In the postfix notation, the operator is placed after the operands, as we will see below this removes the need to define parenthesis for most ordinary operators. For example, instead of writing ‘5+6’, we write ‘5 6 +’. To easily understand how this notation works, you can think of each operand as a node in a first-in-first-out stack. Every time an operator is confronted, it pops the number of operands it needs from the top of the stack (so they don’t exist in the stack any more), does its operation and pushes the result back on top of the stack. So if you want the average of 5 and 6, you would write: ‘5 6 + 2 /’. The operations that are done are: 1. ‘5’ is an operand, so it is pushed to the top of the stack. 2. ‘6’ is an operand, so it is pushed to the top of the stack. 3. ‘+’ is a binary operator, so pull the top two elements of the stack and perform addition on them (the order is ‘5+6’ in the example above). The result is ‘11’, push it on top of the stack. 4. ‘2’ is an operand so push it onto the top of the stack. 5. ‘/’ is a binary operator, so pull out the top two elements of the stack (top-most is ‘2’, then ‘11’) and divide the second one by the first. In Gnuastro’s Arithmetic, the operands can be FITS images or numbers. As you can see, very complicated procedures can be created without the need for parenthesis. Even functions which take an arbitrary number of arguments can be defined in this notation. For example the Postscript language(4) (the programming language in Postscript and compiled into PDF files) uses this notation. ---------- Footnotes ---------- (1) (2) (3) (4) See the EPS and PDF part of *note Recognized file types:: for a little more on the Postscript language.  File: gnuastro.info, Node: Arithmetic operators, Next: Invoking astarithmetic, Prev: Reverse polish notation, Up: Arithmetic 6.2.2 Arithmetic operators -------------------------- The recognized operators in Arithmetic are listed below. See *note Reverse polish notation:: for more on how the operators and operands should be ordered on the command-line. The operands to all operators can be a data array (for example a FITS image) or a number, the output will be an array or number according to the inputs. For example a number multiplied by an array will produce an array. The conditional operators will return pixel, or numerical values of 0 (false) or 1 (true). ‘+’ Addition, so “‘4 5 +’†is equivalent to $4+5$. ‘-’ Subtraction, so “‘4 5 -’†is equivalent to $4-5$. ‘*’ Multiplication, so “‘4 5 "*"’†is equivalent to $4\times5$. On the command-line or in scripts, be sure to quote the multiplication sign (for example ‘"*"’). ‘/’ Division, so “‘4 5 /’†is equivalent to $4/5$. ‘abs’ Absolute value of first operand, so “‘4 abs’†is equivalent to $|4|$. ‘pow’ First operand to the power of the second, so “‘4 5 pow’†is equivalent to $4^5$. ‘sqrt’ The square root of the first operand, so “‘4 sqrt’†is equivalent to $\sqrt{4}$. ‘log’ Natural logarithm of first operand, so “‘4 log’†is equivalent to $\ln(4)$. ‘log10’ Base-10 logarithm of first operand, so “‘4 log10’†is equivalent to $\log(4)$. ‘minvalue’ Minimum value in the top operand on the stack, so “‘a.fits min’†will push the the minimum pixel value in this image onto the stack. Therefore this operator is mainly intended for data (for example images), if the top operand is a number, this operator just returns it without any change. So note that when this operator acts on a single image, the output will no longer be an image, but a number. ‘maxvalue’ Maximum value of first operand, similar to ‘minvalue’. ‘min’ If there are several operands (images), each pixel of the output of this operator will be set to the minimum value of all the operands (images) in that pixel. If the operands are all numbers, then their minimum value will be put in the stack. So “‘a.fits b.fits c.fits min’†will produce an image with the same size as the inputs but each output pixel is set to the minimum respective pixel value of the three input images. Important notes: • All the operands must be either images or numbers, they cannot be mixed. • NaN/blank pixels will be ignored, see *note Blank pixels::. • All available operands on the stack will be pulled for this operator to generate its output. So after calling this operator, there will only be one operand on the stack, see *note Reverse polish notation::. ‘max’ Similar to ‘min’, but the pixels of the output will contain the maximum of the respective pixels in all operands in the stack. ‘average’ Similar to ‘min’, but the pixels of the output will contain the average of the respective pixels in all operands in the stack. ‘median’ Similar to ‘min’, but the pixels of the output will contain the median of the respective pixels in all operands in the stack. ‘lt’ Less than: If the second popped (or left operand in infix notation, see *note Reverse polish notation::) value is smaller than the first popped operand, then this function will return a value of 1, otherwise it will return a value of 0. If both operands are images, then all the pixels will be compared with their counterparts in the other image. If only one operand is an image, then all the pixels will be compared with the the single value (number) of the other operand. Finally if both are numbers, then the output is also just one number (0 or 1). ‘le’ Less or equal: similar to ‘lt’ (‘less than’ operator), but returning 1 when the second popped operand is smaller or equal to the first. ‘gt’ Greater than: similar to ‘lt’ (‘less than’ operator), but returning 1 when the second popped operand is greater than the first. ‘ge’ Greater or equal: similar to ‘lt’ (‘less than’ operator), but returning 1 when the second popped operand is larger or equal to the first. ‘eq’ Equality: similar to ‘lt’ (‘less than’ operator), but returning 1 when the two popped operands are equal (to double precision floating point accuracy). ‘neq’ Non-Equality: similar to ‘lt’ (‘less than’ operator), but returning 1 when the two popped operands are _not_ equal (to double precision floating point accuracy). ‘isblank’ Test for a blank value (see *note Blank pixels::). In essence, this is very similar to the conditional operators: the output is either 1 or 0 (see the ‘less than’ operator above). The difference is that it only needs one operand. Because of the definition of a blank pixel, a blank value is not even equal to itself, so you cannot use the equal operator above to select blank pixels. See the “Blank pixels†box below for more on Blank pixels in Arithmetic. ‘and’ Logical AND: returns 1 if both operands have a non-zero value and 0 if both are zero. Both operands have to be the same kind: either both images or both numbers. ‘or’ Logical OR: returns 1 if either one of the operands is non-zero and 0 only when both operators are zero. Both operands have to be the same kind: either both images or both numbers. ‘not’ Logical NOT: returns 1 when the operand is zero and 0 when the operand is non-zero. The operand can be an image or number, for an image, it is applied to each pixel separately. ‘where’ Change the input (pixel) value ‘where’ a certain condition holds. The conditional operators above can be used to define the condition. Three operands are required for ‘where’. The input format is demonstrated in this simplified example: $ astarithmetic in.fits condition.fits new.fits where The third and second popped operands (‘in.fits’ and ‘condition.fits’ above, see *note Reverse polish notation::) have to be images or all three operands have to be numbers. In the former case (when the first two are images), the third operand can be an image or a number. The value of any pixel in ‘in.fits’ that corresponds to a non-zero pixel of ‘condition.fits’ will be changed to the value of the same pixel in ‘new.fits’ (or a fixed number if the first popped operand is a number). Commonly you won’t be dealing with an actual FITS file of a conditional image. You will probably define the condition in the same run based on some other reference image and use the conditional and logical operators above to make a true/false (or one/zero) image for you internally. For example the case below: $ astarithmetic in.fits reference.fits 100 gt new.fits where *Important reminder for multiplication:* please quote the ‘*’ sign (for example, ‘"*"’ or ‘'*'’). Without quotation, the shell will replace ‘*’ with a list of all the files in your working directory which can produce unpredictable outputs. In any case, the input images are not affected, they are only read. *Blank pixels in Arithmetic:* Currently all Arithmetic operations are internally done in double precision floating points. So all blank pixels in the image (see *note Blank pixels::) will be stored as IEEE NaN values. One particular aspect of NaN values is that by definition they will fail on _any_ comparison. Hence both equal and not-equal operators will fail when both their operands are NaN! The only way to select blank pixels is through the ‘isblank’ operator explained above. One way you can exploit this property of the NaN value to your advantage is when you want a fully zero-valued image (even over the blank pixels) based on an already existing image (with same size and world coordinate system settings). The following command will produce this for you: $ astarithmetic input.fits nan eq --output=all-zeros.fits Note that on the command-line you can write NaN in any case (for example ‘NaN’, or ‘NAN’ are also acceptable). Reading NaN as a floating point number in Gnuastro isn’t case-sensitive. gnuastro-0.2.33-8a3b/doc/gnuastro.info0000644000175000017500000004000013004464701014372 00000000000000This is gnuastro.info, produced by makeinfo version 6.3 from gnuastro.texi. This book documents version 0.2.33-8a3b of the GNU Astronomy Utilities (Gnuastro). Gnuastro provides various programs and libraries for astronomical data manipulation and analysis. Copyright © 2015-2016 Free Software Foundation, Inc. Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled “GNU Free Documentation Licenseâ€. INFO-DIR-SECTION Astronomy START-INFO-DIR-ENTRY * Gnuastro: (gnuastro). GNU Astronomy Utilities. * help-gnuastro: (gnuastro)help-gnuastro mailing list. Getting help. * bug-gnuastro: (gnuastro)Report a bug. How to report bugs * ConvertType: (gnuastro)ConvertType. Convert different file types. * astconvertt: (gnuastro)Invoking astconvertt. Options to ConvertType. * Convolve: (gnuastro)Convolve. Convolve an input file with kernel. * astconvolve: (gnuastro)Invoking astconvolve. Options to Convolve. * CosmicCalculator: (gnuastro)CosmicCalculator. For cosmological params. * astcosmiccal: (gnuastro)Invoking astcosmiccal. Options to CosmicCalculator. * Header: (gnuastro)Header. Print and manipulate data header info. * astheader: (gnuastro)Invoking astheader. Options to Header. * ImageCrop: (gnuastro)ImageCrop. Crop region(s) from image(s). * astimgcrop: (gnuastro)Invoking astimgcrop. Options to ImageCrop. * Arithmetic: (gnuastro)Arithmetic. Arithmetic operations on pixels. * astarithmetic: (gnuastro)Invoking astarithmetic. Options to Arithmetic. * ImageStatistics: (gnuastro)ImageStatistics. Get image Statistics. * astimgstat: (gnuastro)Invoking astimgstat. Options to ImageStatistics. * ImageWarp: (gnuastro)ImageWarp. Warp an image to a new grid. * astimgwarp: (gnuastro)Invoking astimgwarp. Options to ImageWarp. * MakeCatalog: (gnuastro)MakeCatalog. Make a catalog from labeled image. * astmkcatalog: (gnuastro)Invoking astmkcatalog. Options to MakeCatalog. * MakeNoise: (gnuastro)MakeNoise. Make (add) noise to an image. * astmknoise: (gnuastro)Invoking astmkprof. Options to MakeNoise. * MakeProfiles: (gnuastro)MakeProfiles. Make mock profiles. * astmkprof: (gnuastro)Invoking astmkprof. Options to MakeProfiles. * NoiseChisel: (gnuastro)NoiseChisel. Detect signal in noise. * astnoisechisel: (gnuastro)Invoking astnoisechisel. Options to NoiseChisel. * SubtractSky: (gnuastro)SubtractSky. Find and subtract the sky value. * astsubtractsky: (gnuastro)Invoking astsubtractsky. Options to SubtractSky. * Table: (gnuastro)Table. Read and write FITS binary or ASCII tables. * asttable: (gnuastro)Invoking asttable. Options to Table. END-INFO-DIR-ENTRY  Indirect: gnuastro.info-1: 2909 gnuastro.info-2: 311280 gnuastro.info-3: 603189  Tag Table: (Indirect) Node: Top2909 Node: Introduction18849 Node: Quick start21557 Node: Science and its tools23327 Ref: Science and its tools-Footnote-132628 Ref: Science and its tools-Footnote-232688 Ref: Science and its tools-Footnote-332742 Ref: Science and its tools-Footnote-432887 Ref: Science and its tools-Footnote-533022 Node: Your rights33125 Ref: Your rights-Footnote-135447 Node: Naming convention35556 Node: Version numbering36701 Ref: Version numbering-Footnote-139778 Node: GNU Astronomy Utilities 1.040082 Ref: GNU Astronomy Utilities 1.0-Footnote-142023 Node: New to GNU/Linux?42055 Node: Command-line interface44019 Ref: Command-line interface-Footnote-149794 Ref: Command-line interface-Footnote-249826 Ref: Command-line interface-Footnote-349928 Node: Report a bug50164 Ref: Report a bug-Footnote-156019 Ref: Report a bug-Footnote-256082 Node: Suggest new feature56144 Node: Announcements59053 Node: Conventions59534 Node: Acknowledgments61084 Node: Tutorials63204 Ref: Tutorials-Footnote-164824 Node: Hubble visually checks and classifies his catalog65463 Ref: Hubble visually checks and classifies his catalog-Footnote-174334 Ref: Hubble visually checks and classifies his catalog-Footnote-274694 Ref: Hubble visually checks and classifies his catalog-Footnote-374934 Ref: Hubble visually checks and classifies his catalog-Footnote-475085 Ref: Hubble visually checks and classifies his catalog-Footnote-575329 Node: Sufi simulates a detection75375 Ref: Sufi simulates a detection-Footnote-192781 Ref: Sufi simulates a detection-Footnote-293075 Node: Installation93453 Node: Dependencies94990 Node: Mandatory dependencies96368 Node: GNU Scientific Library98509 Node: CFITSIO99295 Ref: CFITSIO-Footnote-1102569 Node: WCSLIB102731 Ref: WCSLIB-Footnote-1104267 Ref: WCSLIB-Footnote-2104401 Node: Optional dependencies104487 Node: Bootstrapping dependencies107104 Ref: Bootstrapping dependencies-Footnote-1113222 Ref: Bootstrapping dependencies-Footnote-2113495 Ref: Bootstrapping dependencies-Footnote-3113957 Ref: Bootstrapping dependencies-Footnote-4114263 Ref: Bootstrapping dependencies-Footnote-5114415 Node: Downloading the source114621 Node: Release tarball115605 Node: Version controlled source119085 Ref: Version controlled source-Footnote-1122017 Ref: Version controlled source-Footnote-2122047 Node: Bootstrapping122320 Ref: Bootstrapping-Footnote-1127549 Node: Synchronizing127669 Ref: Synchronizing-Footnote-1131213 Node: Build and install131409 Node: Configuring133124 Node: Gnuastro configure options134784 Node: Installation directory138420 Ref: Installation directory-Footnote-1149992 Ref: Installation directory-Footnote-2150090 Ref: Installation directory-Footnote-3150220 Ref: Installation directory-Footnote-4150303 Ref: Installation directory-Footnote-5150381 Ref: Installation directory-Footnote-6150555 Node: Executable names151211 Node: Configure and build in RAM155112 Node: Tests158880 Node: A4 print book160521 Node: Known issues161919 Ref: Known issues-Footnote-1167609 Ref: Known issues-Footnote-2167648 Node: Common program behavior167836 Node: Command-line169137 Node: Arguments and options170313 Node: Arguments172524 Node: Options174465 Node: Common options180625 Node: Input output181557 Ref: Input output-Footnote-1184043 Node: Operating modes184180 Node: Configuration files190933 Ref: Configuration files-Footnote-1192916 Ref: Configuration files-Footnote-2192985 Node: Configuration file format193206 Node: Configuration file precedence195529 Node: Current directory and User wide197477 Node: System wide198734 Node: Threads in Gnuastro200134 Node: A note on threads201498 Node: How to run simultaneous operations204000 Ref: How to run simultaneous operations-Footnote-1206677 Ref: How to run simultaneous operations-Footnote-2206722 Node: Final parameter values206774 Ref: Final parameter values-Footnote-1210110 Node: Automatic output210162 Node: Getting help212559 Node: --usage215064 Node: --help216421 Node: Man pages220291 Node: Info221122 Node: help-gnuastro mailing list223545 Node: Output headers224615 Node: Extensions and Tables228755 Node: Header230307 Node: Invoking astheader231056 Ref: Invoking astheader-Footnote-1238712 Node: ConvertType239571 Node: Recognized file types240993 Ref: Recognized file types-Footnote-1247157 Node: Color247204 Node: Invoking astconvertt250290 Node: Table260431 Ref: Table-Footnote-1263246 Node: Invoking asttable263640 Node: Image manipulation269914 Node: ImageCrop270732 Node: ImageCrop modes272886 Node: Crop section syntax277643 Node: Blank pixels280584 Node: Invoking astimgcrop282270 Node: astimgcrop options283989 Ref: astimgcrop options-Footnote-1293332 Ref: astimgcrop options-Footnote-2293406 Node: astimgcrop output293454 Node: Arithmetic295730 Node: Reverse polish notation296711 Ref: Reverse polish notation-Footnote-1299266 Ref: Reverse polish notation-Footnote-2299321 Ref: Reverse polish notation-Footnote-3299377 Ref: Reverse polish notation-Footnote-4299441 Node: Arithmetic operators299553 Node: Invoking astarithmetic311280 Ref: Invoking astarithmetic-Footnote-1316875 Node: Convolve316922 Ref: Convolve-Footnote-1319578 Ref: Convolve-Footnote-2319790 Node: Spatial domain convolution320073 Ref: Spatial domain convolution-Footnote-1321318 Node: Convolution process321379 Node: Edges in the spatial domain323599 Ref: Edges in the spatial domain-Footnote-1326679 Ref: Edges in the spatial domain-Footnote-2326775 Node: Frequency domain and Fourier operations326845 Node: Fourier series historical background329610 Ref: epicycle331188 Ref: Fourier series historical background-Footnote-1334392 Ref: Fourier series historical background-Footnote-2334493 Node: Circles and the complex plane334851 Ref: iandtime339356 Ref: Circles and the complex plane-Footnote-1339602 Node: Fourier series339971 Ref: Fourier series-Footnote-1344112 Node: Fourier transform344209 Ref: Fourier transform-Footnote-1347284 Node: Dirac delta and comb347530 Node: Convolution theorem350934 Ref: Convolution theorem-Footnote-1355034 Node: Sampling theorem355095 Ref: samplingfreq357871 Ref: Sampling theorem-Footnote-1361992 Node: Discrete Fourier transform362137 Ref: Discrete Fourier transform-Footnote-1365457 Ref: Discrete Fourier transform-Footnote-2365571 Node: Fourier operations in two dimensions365704 Ref: Fourier operations in two dimensions-Footnote-1368492 Node: Edges in the frequency domain368655 Node: Spatial vs. Frequency domain372350 Node: Convolution kernel373908 Node: Invoking astconvolve377187 Node: ImageWarp383238 Ref: ImageWarp-Footnote-1386730 Ref: ImageWarp-Footnote-2386873 Node: Warping basics387035 Ref: Warping basics-Footnote-1392980 Ref: Warping basics-Footnote-2393076 Ref: Warping basics-Footnote-3393139 Ref: Warping basics-Footnote-4393200 Ref: Warping basics-Footnote-5393250 Node: Merging multiple warpings393505 Node: Resampling394924 Ref: Resampling-Footnote-1399224 Ref: Resampling-Footnote-2399309 Ref: Resampling-Footnote-3399402 Ref: Resampling-Footnote-4399468 Node: Invoking astimgwarp399516 Ref: Invoking astimgwarp-Footnote-1410412 Node: SubtractSky410546 Node: Sky value411987 Ref: Sky value-Footnote-1415029 Ref: Sky value-Footnote-2415139 Ref: Sky value-Footnote-3415459 Node: Finding the sky value415563 Ref: Finding the sky value-Footnote-1417280 Node: Sky value misconceptions417365 Ref: Sky value misconceptions-Footnote-1419601 Ref: Sky value misconceptions-Footnote-2419872 Node: Tiling an image419957 Node: Quantifying signal in a mesh425514 Node: Grid interpolation and smoothing428728 Node: Checking grid values434218 Node: Mesh grid options436632 Node: Mask image441445 Node: Invoking astsubtractsky444796 Node: Image analysis447788 Node: ImageStatistics448387 Node: Histogram and Cumulative Frequency Plot449658 Node: Sigma clipping452276 Node: Mirror distribution455983 Node: Invoking astimgstat460101 Ref: Invoking astimgstat-Footnote-1471805 Node: NoiseChisel471926 Node: Invoking astnoisechisel474491 Node: NoiseChisel options477274 Node: NoiseChisel output499295 Node: MakeCatalog501771 Ref: MakeCatalog-Footnote-1505140 Node: Quantifying data limits505253 Ref: Quantifying data limits-Footnote-1513503 Ref: Quantifying data limits-Footnote-2513573 Ref: Quantifying data limits-Footnote-3513748 Node: Measuring elliptical parameters513819 Node: Invoking astmkcatalog522510 Ref: Invoking astmkcatalog-Footnote-1546980 Node: Adding new columns to MakeCatalog547156 Node: Modeling and fittings552368 Node: MakeProfiles552993 Node: Modeling basics555651 Node: Defining an ellipse556426 Ref: Defining an ellipse-Footnote-1559006 Node: PSF559066 Ref: PSF-Footnote-1563385 Node: Stars563565 Node: Galaxies564217 Ref: Galaxies-Footnote-1565502 Node: Sampling from a function565705 Node: Oversampling570390 Node: If convolving afterwards571756 Node: Flux Brightness and magnitude572957 Ref: Flux Brightness and magnitude-Footnote-1575686 Ref: Flux Brightness and magnitude-Footnote-2575750 Ref: Flux Brightness and magnitude-Footnote-3575957 Ref: Flux Brightness and magnitude-Footnote-4576336 Ref: Flux Brightness and magnitude-Footnote-5576489 Node: Profile magnitude576604 Node: Invoking astmkprof578413 Node: MakeProfiles catalog580119 Node: MakeProfiles options582192 Ref: MakeProfiles options-Footnote-1598499 Node: MakeProfiles output598649 Node: MakeNoise599594 Node: Noise basics603189 Node: Photon counting noise604008 Ref: Photon counting noise-Footnote-1608380 Node: Instrumental noise608488 Node: Final noised pixel value609855 Node: Generating random numbers610286 Ref: Generating random numbers-Footnote-1615107 Ref: Generating random numbers-Footnote-2615209 Ref: Generating random numbers-Footnote-3615280 Node: Invoking astmknoise615615 Node: High-level calculations617828 Node: CosmicCalculator618623 Node: Distance on a 2D curved space620049 Ref: flatplane622489 Ref: sphericalplane625217 Node: Extending distance concepts to 3D631026 Node: Invoking astcosmiccal632527 Node: Libraries635846 Node: Review of library fundamentals637961 Node: Headers640168 Ref: Headers-Footnote-1650359 Ref: Headers-Footnote-2650417 Ref: Headers-Footnote-3650614 Ref: Headers-Footnote-4650731 Ref: Headers-Footnote-5650837 Node: Linking650918 Ref: Linking-Footnote-1660334 Ref: Linking-Footnote-2660525 Ref: Linking-Footnote-3660807 Ref: Linking-Footnote-4660981 Ref: Linking-Footnote-5661237 Node: Summary and example on libraries661331 Node: Automatic linking script665271 Node: Gnuastro library667016 Ref: Gnuastro library-Footnote-1670532 Node: Installation information670671 Ref: Installation information-Footnote-1672585 Node: Array manipulation672640 Node: Bounding box681616 Node: FITS files683565 Node: CFITSIO datatype685323 Node: FITS macros and data structures688263 Node: FITS functions693192 Node: Git wrappers710129 Node: Linked lists711996 Ref: Linked lists-Footnote-1731464 Node: Mesh grid for an image731730 Node: Polygons744035 Node: Qsort functions749319 Node: Spatial convolution752462 Node: Statistical operations754986 Node: Multithreaded programming771587 Ref: Multithreaded programming-Footnote-1774460 Ref: Multithreaded programming-Footnote-2774620 Node: Implementation of pthread_barrier774682 Node: Gnuastro's thread related functions777594 Node: Text table into a C array781057 Node: World Coordinate System784822 Node: Developing788140 Node: Why C790526 Ref: Why C-Footnote-1796143 Ref: Why C-Footnote-2796342 Ref: Why C-Footnote-3796448 Ref: Why C-Footnote-4796494 Ref: Why C-Footnote-5796705 Node: Program design philosophy796750 Ref: Program design philosophy-Footnote-1799360 Ref: Program design philosophy-Footnote-2799468 Node: Gnuastro project webpage799516 Ref: Gnuastro project webpage-Footnote-1803803 Ref: Gnuastro project webpage-Footnote-2803857 Ref: Gnuastro project webpage-Footnote-3803893 Node: Developing mailing lists804018 Node: Coding conventions806273 Ref: Coding conventions-Footnote-1818586 Ref: Coding conventions-Footnote-2818658 Ref: Coding conventions-Footnote-3819059 Ref: Coding conventions-Footnote-4819222 Node: Program source819492 Node: Mandatory source code files820304 Ref: Mandatory source code files-Footnote-1827270 Node: The TEMPLATE program827385 Node: Documentation829857 Node: Building and debugging833805 Node: Test scripts836755 Node: Developer's checklist839243 Node: Contributing to Gnuastro840686 Node: Copyright assignment842693 Node: Commit guidelines846568 Ref: Commit guidelines-Footnote-1851301 Node: Production workflow851364 Ref: Production workflow-Footnote-1854279 Ref: Production workflow-Footnote-2854358 Ref: Production workflow-Footnote-3854441 Node: Forking tutorial854523 Ref: Forking tutorial-Footnote-1859215 Ref: Forking tutorial-Footnote-2859342 Node: Gnuastro programs list859448 Node: Other useful software863133 Node: SAO ds9863624 Ref: SAO ds9-Footnote-1864796 Node: Viewing multiextension FITS864825 Node: PGPLOT868113 Ref: PGPLOT-Footnote-1871709 Node: GNU Free Documentation License871761 Node: Index897122  End Tag Table  Local Variables: coding: utf-8 End: gnuastro-0.2.33-8a3b/doc/genauthors0000755000175000017500000000522012723106172013767 00000000000000#! /bin/sh # # Update/create authors for the documentation. But only when there is a Git # repository. When there is no $(top_srcdir)/.git directory, rely on the # existing authors list. If the authors.texi file has for some reason been # deleted from the non version controlled source, then the book will not be # made (Texinfo will complain about a missing authors.texi). # # Call like this: # genauthors TOP_SRCDIR # # Original author: # Mohammad Akhlaghi # Contributing author(s): # Mosè Giordano # Copyright (C) 2016, Free Software Foundation, Inc. # # Gnuastro is free software: you can redistribute it and/or modify it under # the terms of the GNU General Public License as published by the Free # Software Foundation, either version 3 of the License, or (at your option) # any later version. # # Gnuastro is distributed in the hope that it will be useful, but WITHOUT # ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or # FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for # more details. # # You should have received a copy of the GNU General Public License along # with Gnuastro. If not, see . # Status report echo "Generating authors list for documentation." # Only do the job if a .git directory exists in the top source directory # (recall that this script is also present in the tar-ball with no .git # directory and might be run from there) if [ -d $1/.git ]; then # We will need to import the `.mailmap' file from the source directory # temporarily to correct the changing emails (see the comments in # `.mailmap'). Note that this script is run from within the `doc/' # directory. The original `.mailmap' is in the `TOP_SRCDIR', so even # when the source and build directories are the same, there is no # problem. ln -s $1/.mailmap .mailmap # Do NOT test if authors.texi is newer than ../.git. In some cases the # list of authors is created empty when running make in top directory # (in particular "make -jN" with N > 1), so authors.texi needs to be # recreated anyway. git --git-dir=$1/.git shortlog --numbered --summary --email --no-merges \ | sed -e 's// /' -e 's/@/@@/' -e "s/è/@\`e/" \ | awk '{printf "%s %s (%s, %s)@*\n", $2, $3, $4, $1}' \ > $1/doc/authors.texi # Clean up: rm .mailmap # Check if the authors.texi file was actually written: if [ ! -s $1/doc/authors.texi ]; then echo "authors.texi is empty!" exit 1 fi else echo "No Git repository detected, leaving $1/doc/authors.texi unchanged." fi gnuastro-0.2.33-8a3b/doc/gnuastro.texi0000644000175000017500000322632413003707213014427 00000000000000\input texinfo @c -*-texinfo-*- @c %**start of header @setfilename gnuastro.info @settitle GNU Astronomy Utilities @documentencoding UTF-8 @allowcodebreaks false @c@afourpaper @c %**end of header @include version.texi @include formath.texi @c So dashes and underscores can be used in HTMLs @allowcodebreaks true @c So function output type is printed on first line @deftypefnnewline on @c Use section titles in cross references, not node titles. @xrefautomaticsectiontitle on @c For the indexes: @syncodeindex vr cp @syncodeindex pg cp @c Copyright information: @copying This book documents version @value{VERSION} of the GNU Astronomy Utilities (Gnuastro). Gnuastro provides various programs and libraries for astronomical data manipulation and analysis. Copyright @copyright{} 2015-2016 Free Software Foundation, Inc. @quotation Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled ``GNU Free Documentation License''. @end quotation @end copying @c To include in the info directory. @dircategory Astronomy @direntry * Gnuastro: (gnuastro). GNU Astronomy Utilities. * help-gnuastro: (gnuastro)help-gnuastro mailing list. Getting help. * bug-gnuastro: (gnuastro)Report a bug. How to report bugs * ConvertType: (gnuastro)ConvertType. Convert different file types. * astconvertt: (gnuastro)Invoking astconvertt. Options to ConvertType. * Convolve: (gnuastro)Convolve. Convolve an input file with kernel. * astconvolve: (gnuastro)Invoking astconvolve. Options to Convolve. * CosmicCalculator: (gnuastro)CosmicCalculator. For cosmological params. * astcosmiccal: (gnuastro)Invoking astcosmiccal. Options to CosmicCalculator. * Header: (gnuastro)Header. Print and manipulate data header info. * astheader: (gnuastro)Invoking astheader. Options to Header. * ImageCrop: (gnuastro)ImageCrop. Crop region(s) from image(s). * astimgcrop: (gnuastro)Invoking astimgcrop. Options to ImageCrop. * Arithmetic: (gnuastro)Arithmetic. Arithmetic operations on pixels. * astarithmetic: (gnuastro)Invoking astarithmetic. Options to Arithmetic. * ImageStatistics: (gnuastro)ImageStatistics. Get image Statistics. * astimgstat: (gnuastro)Invoking astimgstat. Options to ImageStatistics. * ImageWarp: (gnuastro)ImageWarp. Warp an image to a new grid. * astimgwarp: (gnuastro)Invoking astimgwarp. Options to ImageWarp. * MakeCatalog: (gnuastro)MakeCatalog. Make a catalog from labeled image. * astmkcatalog: (gnuastro)Invoking astmkcatalog. Options to MakeCatalog. * MakeNoise: (gnuastro)MakeNoise. Make (add) noise to an image. * astmknoise: (gnuastro)Invoking astmkprof. Options to MakeNoise. * MakeProfiles: (gnuastro)MakeProfiles. Make mock profiles. * astmkprof: (gnuastro)Invoking astmkprof. Options to MakeProfiles. * NoiseChisel: (gnuastro)NoiseChisel. Detect signal in noise. * astnoisechisel: (gnuastro)Invoking astnoisechisel. Options to NoiseChisel. * SubtractSky: (gnuastro)SubtractSky. Find and subtract the sky value. * astsubtractsky: (gnuastro)Invoking astsubtractsky. Options to SubtractSky. * Table: (gnuastro)Table. Read and write FITS binary or ASCII tables. * asttable: (gnuastro)Invoking asttable. Options to Table. @end direntry @c Print title information: @titlepage @title GNU Astronomy Utilities @subtitle Astronomical data manipulation and analysis programs and libraries @subtitle for version @value{VERSION}, @value{UPDATED} @author Mohammad Akhlaghi @page Gnuastro (source code and book) authors (sorted by number of commits in project history): @quotation @include authors.texi @end quotation @vskip 0pt plus 1filll @insertcopying @page @quotation @* @* @* @* @* @* @* @* @* For myself, I am interested in science and in philosophy only because I want to learn something about the riddle of the world in which we live, and the riddle of man’s knowledge of that world. And I believe that only a revival of interest in these riddles can save the sciences and philosophy from narrow specialization and from an obscurantist faith in the expert’s special skill, and in his personal knowledge and authority; a faith that so well fits our ‘post-rationalist’ and ‘post-critical’ age, proudly dedicated to the destruction of the tradition of rational philosophy, and of rational thought itself. @author Karl Popper. The logic of scientific discovery. 1959. @end quotation @end titlepage @shortcontents @contents @c Online version top information. @ifnottex @node Top, Introduction, (dir), (dir) @top GNU Astronomy Utilities @insertcopying @ifhtml To navigate easily in this web page, you can use the @code{Next}, @code{Previous}, @code{Up} and @code{Contents} links in the top and bottom of each page. @code{Next} and @code{Previous} will take you to the next or previous topic in the same level, for example from chapter 1 to chapter 2 or vice versa. To go to the sections or subsections, you have to click on the menu entries that are there when ever a sub-component to a title is present. @end ifhtml @end ifnottex @menu * Introduction:: General introduction. * Tutorials:: Tutorials or Cookbooks. * Installation:: Requirements and installation. * Common program behavior:: Common behavior in all programs. * Extensions and Tables:: Tools to operate on extensions and tables. * Image manipulation:: Tools for basic image manipulation. * Image analysis:: Analyze images. * Modeling and fittings:: Make and fit models. * High-level calculations:: Physical calculations. * Libraries:: Use Gnuastro in your own code. * Developing:: The development environment. * Gnuastro programs list:: List and short summary of Gnuastro. * Other useful software:: Installing other useful software. * GNU Free Documentation License:: Full FDL text. * Index:: Index of terms @detailmenu --- The Detailed Node Listing --- Introduction * Quick start:: A quick start to installation. * Science and its tools:: Some philosophy and history. * Your rights:: User rights. * Naming convention:: About names of programs in Gnuastro. * Version numbering:: Understanding version numbers. * New to GNU/Linux?:: Suggested GNU/Linux distribution. * Report a bug:: Search and report the bug you found. * Suggest new feature:: How to suggest a new feature. * Announcements:: How to stay up to date with Gnuastro. * Conventions:: Conventions used in this book. * Acknowledgments:: People who helped in the production. Version numbering * GNU Astronomy Utilities 1.0:: Plans for version 1.0 release New to GNU/Linux? * Command-line interface:: Introduction to the command-line Tutorials * Hubble visually checks and classifies his catalog:: Check a catalog. * Sufi simulates a detection:: Simulating a detection. Installation * Dependencies:: Necessary packages for Gnuastro. * Downloading the source:: Ways to download the source code. * Build and install:: Configure, build and install Gnuastro. Dependencies * Mandatory dependencies:: Gnuastro will not install without these. * Optional dependencies:: Adding more functionality. * Bootstrapping dependencies:: If you have the version controlled source. Mandatory dependencies * GNU Scientific Library:: Installing GSL. * CFITSIO:: C interface to the FITS standard. * WCSLIB:: C interface to the WCS standard of FITS. Downloading the source * Release tarball:: Download a stable official release. * Version controlled source:: Get and use the version controlled source. Version controlled source * Bootstrapping:: Adding all the automaticly generated files. * Synchronizing:: Keep your local clone up to date. Build and install * Configuring:: Configure Gnuastro * Tests:: Run tests to see if it is working. * A4 print book:: Customize the print book. * Known issues:: Issues you might encounter. Configuring * Gnuastro configure options:: Configure options particular to Gnuastro. * Installation directory:: Specify the directory to install. * Executable names:: Changing executable names. * Configure and build in RAM:: For minimal use of HDD or SSD, and clean source. Common program behavior * Command-line:: How to use the command-line. * Configuration files:: Values for unspecified variables. * Threads in Gnuastro:: How threads are managed in Gnuastro. * Final parameter values:: The final set of used parameters. * Automatic output:: About automatic output names. * Getting help:: Getting more information on the go. * Output headers:: Common headers to all FITS outputs. Command-line * Arguments and options:: Basics of options and arguments. * Arguments:: Treatment of arguments. * Options:: How to use GNU style options. * Common options:: Common options to all Gnuastro programs. Common options * Input output:: Common input/output options. * Operating modes:: Common operating mode options. Configuration files * Configuration file format:: ASCII format of configuration file. * Configuration file precedence:: Precedence of configuration files. * Current directory and User wide:: Local and user configuration files. * System wide:: System wide configuration files. Threads in Gnuastro * A note on threads:: Caution and suggestion on using threads. * How to run simultaneous operations:: How to run things simultaneously. Getting help * --usage:: View option names and value formats. * --help:: List all options with description. * Man pages:: Man pages generated from --help. * Info:: View complete book in terminal. * help-gnuastro mailing list:: Contacting experienced users. Extensions and Tables * Header:: Print and manipulate data file header. * ConvertType:: Convert data to various formats. * Table:: Read and Write FITS tables to plain text. Header * Invoking astheader:: Arguments and options to Header. ConvertType * Recognized file types:: Recognized file types * Color:: Some explanations on color. * Invoking astconvertt:: Options and arguments to ConvertType. Table * Invoking asttable:: Options and arguments to Table. Image manipulation * ImageCrop:: Crop region(s) from FITS image(s). * Arithmetic:: Arithmetic on input data. * Convolve:: Convolve an image with a kernel. * ImageWarp:: Warp/Transform an image to a different grid. * SubtractSky:: Find the sky and subtract it from image. ImageCrop * ImageCrop modes:: Basic ImageCrop modes. * Crop section syntax:: How to define a section to crop. * Blank pixels:: Pixels with no value. * Invoking astimgcrop:: Calling ImageCrop on the command-line Invoking ImageCrop * astimgcrop options:: A list of all the options with explanation. * astimgcrop output:: The outputs of ImageCrop. Arithmetic * Reverse polish notation:: The current notation style for Arithmetic * Arithmetic operators:: List of operators known to Arithmetic * Invoking astarithmetic:: How to run Arithmetic: options and output Convolve * Spatial domain convolution:: Only using the input image values. * Frequency domain and Fourier operations:: Using frequencies in input. * Spatial vs. Frequency domain:: When to use which? * Convolution kernel:: How to specify the convolution kernel. * Invoking astconvolve:: Options and argument to Convolve. Spatial domain convolution * Convolution process:: More basic explanations. * Edges in the spatial domain:: Dealing with the edges of an image. Frequency domain and Fourier operations * Fourier series historical background:: Historical background. * Circles and the complex plane:: Interpreting complex numbers. * Fourier series:: Fourier Series definition. * Fourier transform:: Fourier Transform definition. * Dirac delta and comb:: Dirac delta and Dirac comb. * Convolution theorem:: Derivation of Convolution theorem. * Sampling theorem:: Sampling theorem (Nyquist frequency). * Discrete Fourier transform:: Derivation and explanation of DFT. * Fourier operations in two dimensions:: Extend to 2D images. * Edges in the frequency domain:: Interpretation of edge effects. ImageWarp * Warping basics:: Basics of coordinate transformation. * Merging multiple warpings:: How to merge multiple matrices. * Resampling:: Warping an image is re-sampling it. * Invoking astimgwarp:: Arguments and options for ImageWarp. SubtractSky * Sky value:: Definition of the sky value. * Tiling an image:: Defining a mesh grid on the image. * Mask image:: How to mask pixels for no analysis. * Invoking astsubtractsky:: Options and arguments to SubtractSky. Sky value * Finding the sky value:: How SubtractSky finds the sky value. * Sky value misconceptions:: Sky value misconceptions and wrong approaches. Tiling an image * Quantifying signal in a mesh:: Good meshs for gradients. * Grid interpolation and smoothing:: Filling the blank grid elements. * Checking grid values:: Check the values on the grid. * Mesh grid options:: Common options related to the mesh grid. Image analysis * ImageStatistics:: Calculate main image statistics. * NoiseChisel:: Detect objects in an image. * MakeCatalog:: Catalog from input and labeled images. ImageStatistics * Histogram and Cumulative Frequency Plot:: Basic definitions. * Sigma clipping:: Definition of @mymath{\sigma}-clipping * Mirror distribution:: Used for finding the mode. * Invoking astimgstat:: Arguments and options to ImageStatistics. NoiseChisel * Invoking astnoisechisel:: Options and arguments for NoiseChisel. Invoking NoiseChisel * NoiseChisel options:: The options specific to NoiseChisel. * NoiseChisel output:: NoiseChisel's output. Why no catalog? MakeCatalog * Quantifying data limits:: For comparing different catalogs. * Measuring elliptical parameters:: Estimating elliptical parameters. * Invoking astmkcatalog:: Options and arguments to MakeCatalog. * Adding new columns to MakeCatalog:: How to add new columns. Modeling and fitting * MakeProfiles:: Making mock galaxies and stars. * MakeNoise:: Make (add) noise to an image. MakeProfiles * Modeling basics:: Astronomical modeling basics. * If convolving afterwards:: Considerations for convolving later. * Flux Brightness and magnitude:: About these measures of energy. * Profile magnitude:: Definition of total profile magnitude. * Invoking astmkprof:: Inputs and Options for MakeProfiles. Modeling basics * Defining an ellipse:: Defining an ellipse in 2D. * PSF:: Radial profiles for the PSF. * Stars:: Making mock star profiles. * Galaxies:: Radial profiles for galaxies. * Sampling from a function:: Sample a function on a pixelated canvas. * Oversampling:: Oversampling the model. Invoking MakeProfiles * MakeProfiles catalog:: Required catalog properties. * MakeProfiles options:: Full list of MakeProfiles options. * MakeProfiles output:: The generated outputs. MakeNoise * Noise basics:: Noise concepts and definitions. * Invoking astmknoise:: Options and arguments to MakeNoise. Noise basics * Photon counting noise:: Poisson noise * Instrumental noise:: Readout, dark current and other sources. * Final noised pixel value:: How the final noised value is calculated. * Generating random numbers:: How random numbers are generated. High-level calculations * CosmicCalculator:: Calculate cosmological variables CosmicCalculator * Distance on a 2D curved space:: Distances in 2D for simplicity * Extending distance concepts to 3D:: Going to 3D (our real universe). * Invoking astcosmiccal:: How to run CosmicCalculator Libraries * Review of library fundamentals:: Guide on libraries and linking. * Gnuastro library:: Description of all library functions. Review of library fundamentals * Headers:: Header files included in source. * Linking:: Linking the compiled source files into one. * Summary and example on libraries:: A summary and example on using libraries. * Automatic linking script:: Shell function for automatic linking. Gnuastro library * Installation information:: General information about the installation. * Array manipulation:: Functions for manipulating arrays. * Bounding box:: Finding the bounding box. * FITS files:: Working with FITS data. * Git wrappers:: Wrappers for functions in libgit2. * Linked lists:: Various types of linked lists. * Mesh grid for an image:: Breaking an image into a grid. * Polygons:: Working with the vertices of a polygon. * Qsort functions:: Helper functions for Qsort. * Spatial convolution:: Doing spatial convolution on an image * Statistical operations:: Functions for basic statistics. * Multithreaded programming:: Facilitating use of pthreads. * Text table into a C array:: Read an ASCII text table into a C array. * World Coordinate System:: Dealing with the world coordinate system. FITS files (@file{fits.h}) * CFITSIO datatype:: Addressing different types of data * FITS macros and data structures:: Gnuastro FITS related macros and structures. * FITS functions:: Functions to work on FITS data. Multithreaded programming (@file{threads.h}) * Implementation of pthread_barrier:: Some systems don't have pthread_barrier * Gnuastro's thread related functions:: Functions for managing threads. Developing * Why C:: Why Gnuastro is designed in C. * Program design philosophy:: General ideas behind the package structure. * Gnuastro project webpage:: Central hub for Gnuastro activities. * Developing mailing lists:: Stay up to date with Gnuastro's development. * Coding conventions:: Gnuastro coding conventions. * Program source:: Conventions for the code. * Documentation:: Documentation is an integral part of Gnuastro. * Building and debugging:: Build and possibly debug during development. * Test scripts:: Understanding the test scripts. * Developer's checklist:: Checklist to finalize your changes. * Contributing to Gnuastro:: Share your changes with all users. Program source * Mandatory source code files:: Description of files common to all programs. * The TEMPLATE program:: Template for easy creation of a new program. Contributing to Gnuastro * Copyright assignment:: Copyright has to be assigned to the FSF. * Commit guidelines:: Guidelines for commit messages. * Production workflow:: Submitting your commits (work) for inclusion. * Forking tutorial:: Tutorial on workflow steps with Git. Other useful software * SAO ds9:: Viewing FITS images. * PGPLOT:: Plotting directly in C SAO ds9 * Viewing multiextension FITS:: Configure SAO ds9 for multiextension images. @end detailmenu @end menu @node Introduction, Tutorials, Top, Top @chapter Introduction @cindex GNU coding standards @cindex GNU Astronomy Utilities (Gnuastro) GNU Astronomy Utilities (Gnuastro) is an official GNU package consisting of separate programs and libraries for the manipulation and analysis of astronomical data. All the programs share the same basic command-line user interface for the comfort of both the users and developers. Gnuastro is written to comply fully with the GNU coding standards so it integrates finely with the GNU/Linux operating system. This also enables astronomers to expect a fully familiar experience in the source code, building, installing and command-line user interaction that they have seen in all the other GNU software that they use. The official and always up to date version of this book (or manual) is freely available under @ref{GNU Free Documentation License} in various formats (pdf, html, plain text, info, and as its Texinfo source) at @url{http://www.gnu.org/software/gnuastro/manual/}. For users who are new to the GNU/Linux environment, unless otherwise specified most of the topics in @ref{Installation} and @ref{Common program behavior} are common to all GNU software, for example installation, managing command-line options or getting help (also see @ref{New to GNU/Linux?}). So if you are new to this empowering environment, we encourage you to go through these chapters carefully. They can be a starting point from which you can continue to learn more from each program's own manual and fully benefit from and enjoy this wonderful environment. Gnuastro also comes with a large set of libraries, so you can write your own programs using Gnuastro's building blocks, see @ref{Review of library fundamentals} for an introduction. Finally it must be mentioned that in Gnuastro, no change to any program will be released before it has been fully documented in this here first. As discussed in @ref{Science and its tools} this is the founding basis of the Gnuastro. @menu * Quick start:: A quick start to installation. * Science and its tools:: Some philosophy and history. * Your rights:: User rights. * Naming convention:: About names of programs in Gnuastro. * Version numbering:: Understanding version numbers. * New to GNU/Linux?:: Suggested GNU/Linux distribution. * Report a bug:: Search and report the bug you found. * Suggest new feature:: How to suggest a new feature. * Announcements:: How to stay up to date with Gnuastro. * Conventions:: Conventions used in this book. * Acknowledgments:: People who helped in the production. @end menu @node Quick start, Science and its tools, Introduction, Introduction @section Quick start @cindex Test @cindex Check @cindex Build @cindex Compile @cindex GNU Tar @cindex Uncompress source @cindex Source, uncompress Gnuastro has three mandatory dependencies and two optional ones for added functionality, see @ref{Dependencies}. The latest official release tarball is always available as @url{http://ftp.gnu.org/gnu/gnuastro/gnuastro-latest.tar.gz, @file{gnuastro-latest.tar.gz}}. For better compression (faster download), we also provide an Lzip compressed tarball at @url{http://ftp.gnu.org/gnu/gnuastro/gnuastro-latest.tar.lz, @file{gnuastro-latest.tar.lz}}, see @ref{Release tarball} for more details on the tarball release. If you have downloaded the tarball in the @file{TOPGNUASTRO} directory and the dependencies are installed, you can unpack, compile, check and install Gnuastro with the following commands. If you use GNU Tar, the same command (@command{$ tar xf}) can also be used to unpack @file{.tar.lz} tarballs. @example $ cd TOPGNUASTRO $ tar xf gnuastro-latest.tar.gz # This works on `.tar.lz' too. $ cd gnuastro-X.X # Replace X.X with version number. $ ./configure $ make $ make check $ sudo make install @end example @noindent See @ref{Known issues} if you confront any complications. For each program there is an `Invoke ProgramName' sub-section in this book which explains how the programs should be run on the command-line. You can read it on the command-line by running the command @command{$ info astprogname}, see @ref{Naming convention} and @ref{Getting help}. The `Invoke ProgramName' sub-section starts with a few examples of each program and goes on to explain the invocation details. In @ref{Tutorials} some real life examples of how these programs might be used are given. @node Science and its tools, Your rights, Quick start, Introduction @section Science and its tools History of science indicates that there are always inevitably unseen faults, hidden assumptions, simplifications and approximations in all our theoretical models, data acquisition and analysis techniques. It is precisely these that will ultimately allow future generations to advance the existing experimental and theoretical knowledge through their new solutions and corrections. In the past, scientists would gather data and process them individually to achieve an analysis thus having a much more intricate knowledge of the data and analysis. The theoretical models also required little (if any) simulations to compare with the data. Today both methods are becoming increasingly more dependent on pre-written software. Scientists are dissociating themselves from the intricacies of reducing raw observational data in experimentation or from bringing the theoretical models to life in simulations. These `intricacies' are precisely those unseen faults, hidden assumptions, simplifications and approximations that define scientific progress. @quotation @cindex Anscombe F. J. Unfortunately, most persons who have recourse to a computer for statistical analysis of data are not much interested either in computer programming or in statistical method, being primarily concerned with their own proper business. Hence the common use of library programs and various statistical packages. ... It's time that was changed. @author F. J. Anscombe. The American Statistician, Vol. 27, No. 1. 1973 @end quotation @cindex Anscombe's quartet @cindex Statistical analysis Anscombe's quartet @footnote{@url{http://en.wikipedia.org/wiki/Anscombe%27s_quartet}} demonstrates how four data sets with widely different shapes (when plotted) give nearly identical output from standard regression techniques. Anscombe argues that ``Good statistical analysis is not a purely routine matter, and generally calls for more than one pass through the computer''. Anscombe's quartet can be generalized to say that users of a software cannot claim to understand how it works only based on the experience they have gained by frequently using it. This kind of subjective experience is prone to very serious mis-understandings about what it really does behind the scenes and can be misleading. This attitude is further encouraged through non-free software@footnote{@url{https://www.gnu.org/philosophy/free-sw.html}}. This approach to scientific software only helps in producing dogmas and an ``obscurantist faith in the expert’s special skill, and in his personal knowledge and authority''@footnote{Karl Popper. The logic of scientific discovery. 1959. Larger quote is given at the start of the PDF (for print) version of this book.}. @quotation @cindex Douglas Rushkoff Program or be programmed. Choose the former, and you gain access to the control panel of civilization. Choose the latter, and it could be the last real choice you get to make. @author Douglas Rushkoff. Program or be programmed, O/R Books (2010). @end quotation It is obviously impractical for any one human being to gain the intricate knowledge explained above for every step of an analysis. On the other hand, scientific data can be very large and numerous, for example images produced by telescopes in astronomy. This requires very efficient algorithms. To make things worse, natural scientists have generally not been trained in the advanced software techniques, paradigms and architecture that are taught in computer science or engineering courses and thus used in most software. The GNU Astronomy Utilities are an effort to tackle this issue. Gnuastro is not just a software, this book is as important to the idea behind Gnuastro as the source code (software). This book has tried to learn from the success of the ``Numerical Recipes'' book in educating those who are not software engineers and computer scientists but still heavy users of computational algorithms, like astronomers. There are two major differences: the code and the explanations are segregated: the code is moved within the actual Gnuastro software source code and the underlying explanations are given here. In the source code every non-trivial step is heavily commented and correlated with this book, it follows the same logic of this book, and all the programs follow a similar internal data, function and file structure, see @ref{Program source}. Complementing the code, this book focuses on thoroughly explaining the concepts behind those codes (history, mathematics, science, software and usage advise when necessary) along with detailed instructions on how to run the programs. At the expense of frustrating ``professionals'' or ``experts'', this book and the comments in the code also intentionally avoid jargon and abbreviations. The source code and this book are thus intimately linked, and when considered as a single entity can be thought of as a real (an actual software accompanying the algorithms) ``Numerical Recipes'' for astronomy. The other major and arguably more important difference is that ``Numerical Recipes'' does not allow you to distribute any code that you have learned from it and the book is not freely available. So while it empowers the privileged individual who has access to it, it exacerbates social ignorance. For example it does not allow you to release your software's source code if you have used their codes, you can only publicly release binaries (a black box) to the community. Exactly at the opposite end of the spectrum, Gnuastro's source code is released under the GNU general public license (GPL) and this book is released under the GNU free documentation license. You are therefore free to distribute any software you create using parts of Gnuastro's source code or text, or figures from this book, see @ref{Your rights}. While developing the source code and this book together, the developers of Gnuastro aim to impose the minimum requirements on you (in computer science, engineering and even the mathematics behind the tools) to understand and modify any step of Gnuastro if you feel the need to do so, see @ref{Why C} and @ref{Program design philosophy}. @cindex Galileo, G. Imagine if Galileo did not have the technical knowledge to build a telescope. Astronomical objects could not be seen with the Dutch military design of the telescope. In the beginning of his ``The Sidereal Messenger'' (1610) he cautions the readers on this issue and instructs them on how to build a suitable instrument: without a detailed description of ``how'' he made his observations, no one would believe him. The same is true today, science cannot progress with a black box. Before he actually saw the moons of Jupiter, the mountains on the Moon or the crescent of Venus, he was an anti-Copernican and was “evasive†to Kepler@footnote{Galileo G. (Translated by Maurice A. Finocchiaro). @emph{The essential Galileo}. Hackett publishing company, first edition, 2008.}. Science is not independent of its tools. @cindex Ken Thomson @cindex Stroustrup, Bjarne Bjarne Stroustrup (creator of the C++ language) says: ``Without understanding software, you are reduced to believing in magic''. Ken Thomson (the designer or the Unix operating system) says ``I abhor a system designed for the `user' if that word is a coded pejorative meaning `stupid and unsophisticated'.'' Certainly no scientist (user of a scientific software) would want to be considered a believer in magic, or `stupid and unsophisticated'. However, this can happen when scientists get too distant from the raw data and are mainly indulging themselves in their own high-level (abstract) models (creations). For example, roughly 5 years before special relativity and about two decades before quantum mechanics fundamentally changed Physics, Kelvin is quoted as saying: @quotation @cindex Lord Kelvin @cindex William Thomson There is nothing new to be discovered in physics now. All that remains is more and more precise measurement. @author William Thomson (Lord Kelvin), 1900 @end quotation @noindent A few years earlier, in a speech Albert. A. Michelson said: @quotation @cindex Albert. A. Michelson @cindex Michelson, Albert. A. The more important fundamental laws and facts of physical science have all been discovered, and these are now so firmly established that the possibility of their ever being supplanted in consequence of new discoveries is exceedingly remote.... Our future discoveries must be looked for in the sixth place of decimals. @author Albert. A. Michelson, dedication of Ryerson Physics Lab, U. Chicago 1894 @end quotation @cindex Puzzle solving scientist @cindex Scientist, puzzle solver If scientists are considered to be more than mere ``puzzle solvers''@footnote{Thomas S. Kuhn. @emph{The Structure of Scientific Revolutions}, University of Chicago Press, 1962.} (simply adding to the decimals of known values or observing a feature in 10, 100, or 100000 more galaxies or stars, as Kelvin and Michelson clearly believed), they cannot just passively sit back and uncritically repeat the previous (observational or theoretical) methods/tools on new data. Today there is a wealth of raw telescope images ready (mostly for free) at the finger tips of anyone who is interested with a fast enough internet connection to download them. The only thing lacking is new ways to analyze this data and dig out the treasure that is lying hidden in them to existing methods and techniques. @quotation @cindex Jaynes E. T. New data that we insist on analyzing in terms of old ideas (that is, old models which are not questioned) cannot lead us out of the old ideas. However many data we record and analyze, we may just keep repeating the same old errors, missing the same crucially important things that the experiment was competent to find. @author E. T. Jaynes, Probability theory, the logic of science. 2003. @end quotation @node Your rights, Naming convention, Science and its tools, Introduction @section Your rights @cindex GNU Texinfo The paragraphs below, in this section, belong to the GNU Texinfo@footnote{Texinfo is the GNU documentation system. It is used to create this book in all the various formats.} manual and are not written by us! The name ``Texinfo'' is just changed to ``GNU Astronomy Utilities'' or ``Gnuastro'' because they are released under the same licenses and it is beautifully written to inform you of your rights. @cindex Free software @cindex Copyright @cindex Public domain GNU Astronomy Utilities is ``free software''; this means that everyone is free to use it and free to redistribute it on certain conditions. Gnuastro is not in the public domain; it is copyrighted and there are restrictions on its distribution, but these restrictions are designed to permit everything that a good cooperating citizen would want to do. What is not allowed is to try to prevent others from further sharing any version of Gnuastro that they might get from you. Specifically, we want to make sure that you have the right to give away copies of the programs that relate to Gnuastro, that you receive the source code or else can get it if you want it, that you can change these programs or use pieces of them in new free programs, and that you know you can do these things. To make sure that everyone has such rights, we have to forbid you to deprive anyone else of these rights. For example, if you distribute copies of the Gnuastro related programs, you must give the recipients all the rights that you have. You must make sure that they, too, receive or can get the source code. And you must tell them their rights. Also, for our own protection, we must make certain that everyone finds out that there is no warranty for the programs that relate to Gnuastro. If these programs are modified by someone else and passed on, we want their recipients to know that what they have is not what we distributed, so that any problems introduced by others will not reflect on our reputation. @cindex GNU General Public License @cindex GNU Free Documentation License The precise conditions of the licenses for the programs currently being distributed that relate to Gnuastro are found in the @url{http://www.gnu.org/copyleft/gpl.html, GNU General Public license} that accompany them. This book is covered by the @url{http://www.gnu.org/copyleft/fdl.html, GNU Free Documentation License}. @node Naming convention, Version numbering, Your rights, Introduction @section Naming convention @cindex Names, programs @cindex Program names Gnuastro is a package of independent programs and a collection of libraries, here we are mainly concerned with the programs. Each program has an official name which consists of one or two words, describing what they do. The latter are printed with no space, for example NoiseChisel or ImageCrop. On the command-line, you can run them with their executable names which start with an @file{ast} and might be an abbreviation of the official name, for example @file{astnoisechisel} or @file{astimgcrop}, see @ref{Executable names}. @pindex ProgramName @pindex @file{astprogname} We will use ``ProgramName'' for a generic official program name and @file{astprogname} for a generic executable name. In this book, the programs are classified based on what they do and thoroughly explained. An alphabetical list of the programs that are installed on your system with this installation are given in @ref{Gnuastro programs list}. That list also contains the executable names and version numbers along with a one line description. @node Version numbering, New to GNU/Linux?, Naming convention, Introduction @section Version numbering @cindex Version number @cindex Number, version @cindex Major version number @cindex Minor version number @cindex Mailing list: info-gnuastro Gnuastro can have two formats of version numbers, for official and unofficial releases. Official Gnuastro releases are announced on the @command{info-gnuastro} mailing list, they have a version control tag in Gnuastro's development history, and their version numbers are formatted like ``@file{A.B}''. @file{A} is a major version number, marking a significant planned achievement (for example see @ref{GNU Astronomy Utilities 1.0}), while @file{B} is a minor version number, see below for more on the distinction. Note that the numbers are not decimals, so version 2.34 is much more recent than version 2.5, which is not equal to 2.50. Gnuastro also allows a unique version number for unofficial releases. Unofficial releases can mark any point in Gnuastro's development history. This is done to allow astronomers to easily use any point in the version controlled history for their data-analysis and research publication. See @ref{Version controlled source} for a complete introduction. This section is not just for developers and is very straightforward, so please have a look if you are interested in the cutting-edge. This unofficial version number is a meaningful and easy to read string of characters, unique to that particular point of history. With this feature, users can easily stay up to date with the most recent bug fixes and additions that are committed between official releases. The unofficial version number is formatted like: @file{A.B.C-D}. @file{A} and @file{B} are the most recent official version number. @file{C} is the number of commits that have been made after version @file{A.B}. @file{D} is the first 4 or 5 characters of the commit hash number@footnote{Each point in Gnuastro's history is uniquely identified with a 40 character long hash which is created from its contents and previous history for example: @code{5b17501d8f29ba3cd610673261e6e2229c846d35}. So the string @file{D} in the version for this commit could be @file{5b17}, or @file{5b175}.}. Therefore, the unofficial version number `@code{3.92.8-29c8}', corresponds to the 8th commit after the official version @code{3.92} and its commit hash begins with @code{29c8}. The unofficial version number is sort-able (unlike the raw hash) and as shown above is very descriptive of the state of the unofficial release. Of course an official release is preferred for publication (since its tarballs are easily available and it has gone through more tests, making it more stable), so if an official release is announced prior to your publication's final review, please consider updating to the official release. The major version number is set by a major goal which is defined by the developers and user community before hand, for example see @ref{GNU Astronomy Utilities 1.0}. The incremental work done in minor releases are commonly small steps in achieving the major goal. Therefore, there is no limit on the number of minor releases and the difference between the (hypothetical) versions 2.927 and 3.0 can be a very small (negligible to the user) improvement that finalizes the defined goals. @menu * GNU Astronomy Utilities 1.0:: Plans for version 1.0 release @end menu @node GNU Astronomy Utilities 1.0, , Version numbering, Version numbering @subsection GNU Astronomy Utilities 1.0 @cindex Gnuastro major version number Currently (prior to Gnuastro 1.0), the aim of Gnuastro is to have a complete system for data manipulation and analysis at least similar to IRAF@footnote{@url{http://iraf.noao.edu/}}. So an astronomer can take all the standard data analysis steps (starting from raw data to the final reduced product and standard post-reduction tools) with the various programs in Gnuastro. @cindex Shell script The maintainers of each camera or detector on a telescope can provide a completely transparent shell script or Makefile to the observer for data analysis. This script can set configuration files for all the required programs to work with that particular camera. The script can then run the proper programs in the proper sequence. The user/observer can easily follow the standard shell script to understand (and modify) each step and the parameters used easily. Bash (or other modern GNU/Linux shell scripts) are very powerful and made for this gluing job. This will simultaneously improve performance and transparency. Shell scripting (or Makefiles) are also very basic constructs that are easy to learn and readily available as part of the Unix-like operating systems. If there is no program to do a desired step, Gnuastro's libraries can be used to build specific programs. The main factor is that all observatories or projects can freely contribute to Gnuastro and all simultaneously benefit from it (since it doesn't belong to any particular one of them), much like how for-profit organizations (for example RedHat, or Intel and many others) are major contributors to free and open source software for their shared benefit. Gnuastro's copyright has been fully awarded to GNU, so it doesn't belong to any particular astronomer or astronomical facility or project. @node New to GNU/Linux?, Report a bug, Version numbering, Introduction @section New to GNU/Linux? Some astronomers initially install and use the GNU/Linux operating systems because the software that their research community use can only be run in this environment, the transition is not necessarily easy. To encourage you in investing the patience and time to make this transition, we define the GNU/Linux system and argue for the command-line interface of scientific software and how it is worth the (apparently steep) learning curve. @ref{Command-line interface} contains a short overview of the very powerful command-line user interface. @ref{Tutorials} is a complete chapter with some real world example applications of Gnuastro making good use of GNU/Linux capabilities written for newcomers to this environment. It is fully explained, easy and (hopefully) entertaining. @cindex Linux @cindex GNU/Linux @cindex GNU C library @cindex GNU Compiler Collection You might have already noticed that we are not using the name ``Linux'', but ``GNU/Linux''. Please take the time to have a look at the following essays and FAQs for a complete understanding of this very important distinction. In short, the Linux kernel is built using the GNU C library (glibc) and GNU compiler collection (gcc). The Linux kernel software alone is useless, in order have an operating system you need many more packages and the majority of such low-level packages in most distributions are developed as part of the GNU project: ``the whole system is basically GNU with Linux loaded''. In the form of an analogy: to say “running Linuxâ€, is like saying “driving your carburetorâ€. @itemize @item @url{https://www.gnu.org/gnu/gnu-users-never-heard-of-gnu.html} @item @url{https://www.gnu.org/gnu/linux-and-gnu.html} @item @url{https://www.gnu.org/gnu/why-gnu-linux.html} @item @url{https://www.gnu.org/gnu/gnu-linux-faq.html} @end itemize @menu * Command-line interface:: Introduction to the command-line @end menu @node Command-line interface, , New to GNU/Linux?, New to GNU/Linux? @subsection Command-line interface @cindex Shell @cindex Graphic user interface @cindex Command-line user interface @cindex GUI: graphic user interface @cindex CLI: command-line user interface One aspect of Gnuastro that might be a little troubling to new GNU/Linux users is that (at least for the time being) it only has a command-line user interface (CLI). This might be contrary to the mostly graphical user interface (GUI) experience with proprietary operating systems. To a first time user, the command-line does appear much more complicated and adapting to it might not be easy and a little frustrating at first. This is understandable and also experienced by anyone who started using the computer (from childhood) in a graphical user interface. Here we hope to convince you of the unique benefits of this interface which can greatly enhance your productivity while complementing your GUI experience. @cindex GNOME 3 Through GNOME 3@footnote{@url{http://www.gnome.org/}}, most GNU/Linux based operating systems now have a very advanced and useful GUI. Since the GUI was created long after the command-line, some wrongly consider the command line to be obsolete. Both interfaces are very useful for different tasks (for example you can't view an image, video, pdf document or web page on the command-line!), on the other hand you can't reproduce your results easily in the GUI. Therefore they should not be regarded as rivals but as complementary user interfaces, here we will outline how the CLI can be useful in scientific programs. You can think of the GUI as a veneer over the CLI to facilitate a small subset of all the possible CLI operations. Each click you do on the GUI, can be thought of as internally running a different CLI command. So asymptotically (if a good designer can design a GUI which is able to show you all the possibilities to click on) the GUI is only as powerful as the command-line. In practice, such graphical designers are very hard to find for every program, so the GUI operations are always a subset of the internal CLI commands. For programs that are only made for the GUI, this results in not including lots of potentially useful operations. It also results in `interface design' to be a crucially important part of any GUI program. Scientists don't usually have enough resources to hire a graphical designer, also the complexity of the GUI code is far more than CLI code, which is harmful for a scientific software, see @ref{Science and its tools}. @cindex GUI: repeating operations For programs that have a GUI, one action on the GUI (moving and clicking a mouse, or tapping a touchscreen) might be more efficient and easier than its CLI counterpart (typing the program name and your desired configuration). However, if you have to repeat that same action more than once, the GUI will soon become very frustrating and prone to errors. Unless the designers of a particular program decided to design such a system for a particular GUI action, there is no general way to run any possible series of actions automatically on the GUI. @cindex GNU Bash @cindex Reproducible results @cindex CLI: repeating operations On the command-line, you can run any series of of actions which can come from various CLI capable programs you have decided your self in any possible permutation with one command@footnote{By writing a shell script and running it, for example see the tutorials in @ref{Tutorials}.}. This allows for much more creativity and exact reproducibility that is not possible to a GUI user. For technical and scientific operations, where the same operation (using various programs) has to be done on a large set of data files, this is crucially important. It also allows exact reproducibility which is a foundation principle for scientific results. The most common CLI (which is also known as a shell) in GNU/Linux is GNU Bash, we strongly encourage you to put aside several hours and go through this beautifully explained web page: @url{https://flossmanuals.net/command-line/}. You don't need to read or even fully understand the whole thing, only a general knowledge of the first few chapters are enough to get you going. Since the operations in the GUI are very limited and they are visible, reading a manual is not that important in the GUI (most programs don't even have any!). However, to give you the creative power explained above, with a CLI program, it is best if you first read the manual of any program you are using. You don't need to memorize any details, only an understanding of the generalities is needed. Once you start working, there are more easier ways to remember a particular option or operation detail, see @ref{Getting help}. @cindex GNU Emacs @cindex Virtual console To experience the command-line in its full glory and not in the GUI terminal emulator, press the following keys together: @key{CTRL+ALT+F4}@footnote{Instead of @key{F4}, you can use any of the keys from @key{F1} to @key{F6} for different virtual consoles depending on your GNU/Linux distribution, try them all out. You can also run a separate GUI from within this console if you want to.} to access the virtual console. To return back to your GUI, press the same keys above replacing @key{F4} with @key{F7} (or @key{F1}, or @key{F2}, depending on your GNU/Linux distribution). In the virtual console, the GUI, with all its distracting colors and information, is gone. Enabling you to focus entirely on your actual work. @cindex Resource heavy operations For operations that use a lot of your system's resources (processing a large number of large astronomical images for example), the virtual console is the place to run them. This is because the GUI is not competing with your research work for your system's RAM and CPU. Since the virtual consoles are completely independent, you can even log out of your GUI environment to give even more of your hardware resources to the programs you are running and thus reduce the operating time. @cindex Secure shell @cindex SSH @cindex Remote operation Since it uses far less system resources, the CLI is also very convenient for remote access to your computer. Using secure shell (SSH) you can log in securely to your system (similar to the virtual console) from anywhere even if the connection speeds are low. There are apps for smart phones and tablets which allow you to do this. @node Report a bug, Suggest new feature, New to GNU/Linux?, Introduction @section Report a bug @cindex Bug @cindex Wrong output @cindex Software bug @cindex Output, wrong @cindex Wrong results @cindex Results, wrong @cindex Halted program @cindex Program crashing @cindex Inconsistent results According to Wikipedia ``a software bug is an error, flaw, failure, or fault in a computer program or system that causes it to produce an incorrect or unexpected result, or to behave in unintended ways''. So when you see that a program is crashing, not reading your input correctly, giving the wrong results, or not writing your output correctly, you have found a bug. In such cases, it is best if you report the bug to the developers. The programs will also report bugs in known impossible situations (which are caused by something unexpected) and will ask the users to report the bug. @cindex Bug reporting Prior to actually filing a bug report, it is best to search previous reports. The issue might have already been found and even solved. The best place to check if your bug has already been discussed is the bugs tracker on @ref{Gnuastro project webpage} at @url{https://savannah.gnu.org/bugs/?group=gnuastro}. In the top search fields (under ``Display Criteria'') set the ``Open/Closed'' drop-down menu to ``Any'' and choose the respective program or general category of the bug in ``Category'' and click the ``Apply'' button. The results colored green have already been solved and the status of those colored in red is shown in the table. @cindex Version control Recently corrected bugs are probably not yet publicly released because they are scheduled for the next Gnuastro stable release. If the bug is solved but not yet released and it is an urgent issue for you, you can get the version controlled source and compile that, see @ref{Version controlled source}. To solve the issue as readily as possible, please follow the following to guidelines in your bug report. The @url{http://www.chiark.greenend.org.uk/~sgtatham/bugs.html, How to Report Bugs Effectively} and @url{http://catb.org/~esr/faqs/smart-questions.html, How To Ask Questions The Smart Way} essays also provide some very good generic advice for all software (don't contact their authors for Gnuastro's problems). Mastering the art of giving good bug reports (like asking good questions) can greatly enhance your experience with any free and open source software. So investing the time to read through these essays will greatly reduce your frustration after you see something doesn't work the way you feel it is supposed to for a large range of software, not just Gnuastro. @table @strong @item Be descriptive Please provide as many details as possible and be very descriptive. Explain what you expected and what the output was: it might be that your expectation was wrong. Also please clearly state which sections of the Gnuastro book (this book), or other references you have studied to understand the problem. This can be useful in correcting the book (adding links to likely places where users will check). But more importantly, it will be very encouraging for the developers, since you are showing how serious you are about the problem and that you have actually put some thought into it. ``To be able to ask a question clearly is two-thirds of the way to getting it answered.'' -- John Ruskin (1819-1900). @item Individual and independent bug reports If you have found multiple bugs, please send them as separate (and independent) bugs (as much as possible). This will significantly help us in managing and resolving them sooner. @cindex Reproducible bug reports @item Reproducible bug reports If we cannot exactly reproduce your bug, then it is very hard to resolve it. So please send us a Minimal working example@footnote{@url{http://en.wikipedia.org/wiki/Minimal_Working_Example}} along with the description. For example in running a program, please send us the full command-line text and the output with the @option{-P} option, see @ref{Final parameter values}. If it is caused only for a certain input, also send us that input file. In case the input FITS is large, please use ImageCrop to only crop the problematic section and make it as small as possible so it can easily be uploaded and downloaded and not waste the archive's storage, see @ref{ImageCrop}. @end table @noindent There are generally two ways to inform us of bugs: @itemize @cindex Mailing list archives @cindex Mailing list: bug-gnuastro @cindex @code{bug-gnuastro@@gnu.org} @item Send a mail to @code{bug-gnuastro@@gnu.org}. Any mail you send to this address will be distributed through the bug-gnuastro mailing list@footnote{@url{https://lists.gnu.org/mailman/listinfo/bug-gnuastro}}. This is the simplest way to send us bug reports. The developers will then register the bug into the project webpage (next choice) for you. @cindex Gnuastro project page @cindex Support request manager @cindex Submit new tracker item @cindex Anonymous bug submission @item Use the Gnuastro project webpage at @url{https://savannah.gnu.org/projects/gnuastro/}: There are two ways to get to the submission page as listed below. Fill in the form as described below and submit it (see @ref{Gnuastro project webpage} for more on the project webpage). @itemize @item Using the top horizontal menu items, immediately under the top page title. Hovering your mouse on ``Support'' will open a drop-down list. Select ``Submit new''. @item In the main body of the page, under the ``Communication tools'' section, click on ``Submit new item''. @end itemize @end itemize @cindex Tracker @cindex Bug tracker @cindex Task tracker @cindex Viewing trackers Once the items have been registered in the mailing list or webpage, the developers will add it to either the ``Bug Tracker'' or ``Task Manager'' trackers of the Gnuastro project webpage. These two trackers can only be edited by the Gnuastro project developers, but they can be browsed by anyone, so you can follow the progress on your bug. You are most welcome to join us in developing Gnuastro and fixing the bug you have found maybe a good starting point. Gnuastro is designed to be easy for anyone to develop (see @ref{Science and its tools}) and there is a full chapter devoted to developing it: @ref{Developing}. @node Suggest new feature, Announcements, Report a bug, Introduction @section Suggest new feature @cindex Feature requests @cindex Additions to Gnuastro We would always be very happy to hear of suggested new features. For every program there are already lists of features that we are planning to add. You can see the current list of plans from the Gnuastro project webpage at @url{https://savannah.gnu.org/projects/gnuastro/} and following @clicksequence{``Tasks''@click{}``Browse''} on the horizontal menu at the top of the page immediately under the title, see @ref{Gnuastro project webpage}. If you want to request a feature to an existing program, click on the ``Display Criteria'' above the list and under ``Category'', choose that particular program. Under ``Category'' you can also see the existing suggestions for new programs or other cases like installation, documentation or libraries. Also be sure to set the ``Open/Closed'' value to ``Any''. If the feature you want to suggest is not already listed in the task manager, then follow the steps that are fully described in @ref{Report a bug}. Please have in mind that the developers are all very busy with their own astronomical research, and implementing existing ``task''s to add or resolving bugs. Gnuastro is a volunteer effort and none of the developers are paid for their hard work. So, although we will try our best, please don't not expect that your suggested feature be immediately included (with the next release of Gnuastro). The best person to apply the exciting new feature you have in mind is you, since you have the motivation and need. In fact Gnuastro is designed for making it as easy as possible for you to hack into it (add new features, change existing ones and so on), see @ref{Science and its tools}. Please have a look at the chapter devoted to developing (@ref{Developing}) and start applying your desired feature. Once you have added it, you can use it for your own work and if you feel you want others to benefit from your work, you can request for it to become part of Gnuastro. You can then join the developers and start maintaining your own part of Gnuastro. If you choose to take this path of action please contact us before hand (@ref{Report a bug}) so we can avoid possible duplicate activities and get interested people in contact. @cartouche @noindent @strong{Gnuastro is a collection of low level programs:} As described in @ref{Program design philosophy}, a founding principle of Gnuastro is that each library or program should be very basic and low-level. High level jobs should be done by running the separate programs or using separate functions in succession through a shell script or calling the libraries by higher level functions, see the examples in @ref{Tutorials}. So when making the suggestions please consider how your desired job can best be broken into separate steps and modularized. @end cartouche @node Announcements, Conventions, Suggest new feature, Introduction @section Announcements @cindex Announcements @cindex Mailing list: info-gnuastro Gnuastro has a dedicated mailing list for making announcements. Anyone that is interested can subscribe to this mailing list to stay up to date with new releases or when the dependencies (see @ref{Dependencies}) have been updated. To subscribe to this list, please visit @url{https://lists.gnu.org/mailman/listinfo/info-gnuastro}. @node Conventions, Acknowledgments, Announcements, Introduction @section Conventions In this book we have the following conventions: @itemize @item All commands that are to be run on the shell (command-line) prompt as the user start with a @command{$}. In case they must be run as a super-user or system administrator, they will start with a @command{#}. If the command is in a separate line and next line @code{is also in the code type face}, but doesn't have any of the @command{$} or @command{#} signs, then it is the output of the command after it is run. As a user, you don't need to type those lines. @item If the command becomes larger than the page width a @key{\} is inserted in the code. If you are typing the code by hand on the command-line, you don't need to use multiple lines or add the extra space characters, so you can omit them. If you want to copy and paste these examples (highly discouraged!) then the @key{\} should stay. The @key{\} character is a shell escape character which is used commonly to make characters which have special meaning for the shell loose that special place (the shell will not treat them specially if there is a @key{\} behind them). When it is a last character in a line (the next character is a new-line character) the new-line character looses its meaning an the shell sees it as a simple white-space character, enabling you to use multiple lines to write your commands. @end itemize @node Acknowledgments, , Conventions, Introduction @section Acknowledgments The list of Gnuastro authors is available at the start of this book and the @file{AUTHORS} file in the source code. Here the authors wish to gratefully acknowledge the help and support they received from other people and institutions who had an indirect (not committed in the version controlled history) role in Gnuastro. The plain text file @file{THANKS} which is distributed along with the source code also contains this list. The Japanese Ministry of Science and Technology (MEXT) scholarship for Mohammad Akhlaghi's Masters and PhD period in Tohoku University Astronomical Institute had an instrumental role in the long term learning and planning that made the idea of Gnuastro possible. The very critical view points of Professor Takashi Ichikawa (from Tohoku University) were also instrumental in the initial ideas and creation of Gnuastro. Brandon Invergo, Karl Berry and Richard Stallman also provided very useful suggestions during the GNU evaluation process. Bob Proulx from Savannah, has kindly supported Gnuastro's project webpage on Savannah and the management of its version controlled source server there. @c To the developers: if you would like to thank someone, please change the @c `and' before the last name to a comma (','), then add " and Firstname @c Familyname'' after the last name. We would also like to gratefully thank Mohammad-reza Khellat, Alan Lefor, Yahya Sefidbakht, Francesco Montanari, and Ole Streicher for their useful and constructive comments and suggestions. Finally we should thank all the (sometimes anonymous) developers in various online forums which patiently answered all our small (but important) technical questions. All work on Gnuastro has been voluntary, but we are most grateful to the following institutions (in chronological order) for hosting us in our research: @quotation Ministry of education, culture, sports, science and technology (MEXT), Japan.@* Tohoku University Astronomical Institute, Sendai, Japan.@* University of Salento, Lecce, Italy.@* Centre national de la recherche scientifique (CNRS), France.@* Centre de Recherche Astrophysique de Lyon, University of Lyon 1, France.@* @end quotation @node Tutorials, Installation, Introduction, Top @chapter Tutorials @cindex Tutorial @cindex Cookbook In this chapter we give several tutorials or cookbooks on how to use the various tools in Gnuastro for your scientific purposes. In these tutorials, we have intentionally avoided too many cross references to make it more easily readable. To get more information about a particular program, you can visit the section with the same name as the program in this book. Each program section starts by explaining the general concepts behind what it does. If you only want to see an explanation of the options and arguments of any program, see the subsection titled `Invoking ProgramName'. See @ref{Conventions}, for an explanation of the conventions we use in the example codes through the book. The tutorials in this section use a fictional setting of some historical figures in the history of astronomy. We have tried to show how Gnuastro would have been helpful for them in making their discoveries if there were GNU/Linux computers in their times! Please excuse us for any historical inaccuracy, this is not intended to be a historical reference. This form of presentation can make the tutorials more pleasant and entertaining to read while also being more practical (explaining from a user's point of view)@footnote{This form of presenting a tutorial was influenced by the PGF/TikZ and Beamer manuals. The first provides graphic capabilities, while with the second you can make presentation slides in @TeX{} and @LaTeX{}. In these manuals, Till Tantau (author of the manual) uses Euclid as the protagonist. There are also some nice words of wisdom for Unix-like systems called ``Rootless Root'': @url{http://catb.org/esr/writings/unix-koans/}. These also have a similar style but they use a mythical figure named Master Foo. If you already have some experience in Unix-like systems, you will definitely find these ``Unix Koans'' very entertaining.}. The main reference for the historical facts mentioned in these fictional settings was Wikipedia. @menu * Hubble visually checks and classifies his catalog:: Check a catalog. * Sufi simulates a detection:: Simulating a detection. @end menu @node Hubble visually checks and classifies his catalog, Sufi simulates a detection, Tutorials, Tutorials @section Hubble visually checks and classifies his catalog @cindex Edwin Hubble In 1924 Hubble@footnote{Edwin Powell Hubble (1889 -- 1953 A.D.) was an American astronomer who can be considered as the father of extra-galactic astronomy, by proving that some nebulae are too distant to be within the Galaxy. He then went on to show that the universe appears to expand and also done a visual classification of the galaxies that is known as the Hubble fork.} announced his discovery that some of the known nebulous objects are too distant to be within the the Milky Way (or Galaxy) and that they were probably distant Galaxies@footnote{Note that at that time, ``Galaxy'' was a proper noun used to refer to the Milky way. The concept of a galaxy as we define it today had not yet become common. Hubble played a major role in creating today's concept of a galaxy.} in their own right. He had also used them to show that the redshift of the nebulae increases with their distance. So now he wants to study them more accurately to see what they actually are. Since they are nebulous or amorphous, they can't be modeled (like stars that are always a point) easily. So there is no better way to distinguish them than to visually inspect them and see if it is possible to classify these nebulae or not. Hubble has stored all the FITS images of the objects he wants to visually inspect in his @file{/mnt/data/images} directory. He has also stored his catalog of extra Galactic nebulae in @file{/mnt/data/catalogs/extragalactic.txt}. Any normal user on his GNU/Linux system (including himself) only has read access to the contents of the @file{/mnt/data} directory. He has done this by running this command as root: @example # chmod -R 755 /mnt/data @end example @noindent Hubble has done this intentionally to avoid mistakenly deleting or modifying the valuable images he has taken at Mount Wilson while he is working as an ordinary user. Retaking all those images and data is simply not an option. In fact they are also in another hard disk (@file{/dev/sdb1}). So if the hard disk which stores his GNU/Linux distribution suddenly malfunctions due to work load, his data is not in harms way. That hard disk is only mounted to this directory when he wants to use it with the command: @example # mount /dev/sdb1 /mnt/data @end example @noindent In short, Hubble wants to keep his data safe and fortunately by default Gnuastro allows for this. Hubble creates a temporary @file{visualcheck} directory in his home directory for this check. He runs the following commands to make the directory and change to it@footnote{The @code{pwd} command is short for ``Print Working Directory'' and @code{ls} is short for ``list'' which shows the contents of a directory.}: @example $ mkdir ~/visualcheck $ cd ~/visualcheck $ pwd /home/edwin/visualcheck $ ls @end example Hubble has multiple images in @file{/mnt/data/images}, some of his targets might be on the edges of an image and so several images need to be stitched to give a good view of them. Also his extra Galactic targets belong to various pointings in the sky, so they are not in one large image. Gnuastro's ImageCrop is just the program he wants. The catalog in @file{extragalactic.txt} is a plain text file which stores the basic information of all his known 200 extra Galactic nebulae. In its second column it has each object's Right Ascension (the first column is a label he has given to each object) and in the third the object's declination. Having read the Gnuastro manual, he knows that all counting is done starting from zero, so the RA and Dec columns have number 1 and 2 respectively. @example $ astimgcrop --racol=1 --deccol=2 /mnt/data/images/*.fits \ /mnt/data/catalogs/extragalactic.txt ImageCrop started on Tue Jun 14 10:18:11 1932 ---- ./4_crop.fits 1 1 ---- ./2_crop.fits 1 1 ---- ./1_crop.fits 1 1 [[[ Truncated middle of list ]]] ---- ./198_crop.fits 1 1 ---- ./195_crop.fits 1 1 - 200 images created. - 200 were filled in the center. - 0 used more than one input. ImageCrop finished in: 2.429401 (seconds) @end example @cindex Asynchronous thread allocation @noindent Hubble already knows that thread allocation to the the CPU cores is asynchronous, so each time you run it the order of which job gets done first differs. When using ImageCrop the order of outputs is irrelevant since each crop is independent of the rest. This is why the crops are not necessarily created in the same input order. He is content with the default width of the outputs (which he inspected by running @code{$ astimgcrop -P}). If he wanted a different width for the cropped images, he could do that with the @option{--wwidth} option which accepts a value in arc-seconds. When he lists the contents of the directory again he finds his 200 objects as separate FITS images. @example $ ls 1_crop.fits 2_crop.fits ... 200_crop.fits @end example @cindex GNU Parallel The FITS image format was not designed for viewing, but mainly for accurate storing of the data. So he chooses to convert the cropped images to a more common image format to view them more quickly and easily through standard image viewers (which load much faster than FITS image viewer). JPEG is one of the most recognized image formats that is supported by most image viewers. Fortunately Gnuastro has just such a tool to convert various types of file types to and from each other: ConvertType. Hubble has already heard of GNU Parallel from one of his colleagues at Mount Wilson Observatory. It allows multiple instances of a command to be run simultaneously on the system, so he uses it in conjunction with ConvertType to convert all the images to JPEG. @example $ parallel astconvertt -ojpg ::: *_crop.fits @end example @pindex eog @cindex Eye of GNOME For his graphical user interface Hubble is using GNOME which is the default in most distributions in GNU/Linux. The basic image viewer in GNOME is the Eye of GNOME, which has the executable file name @command{eog} @footnote{Eye of GNOME is only available for users of the GNOME graphical desktop environment which is the default in most GNU/Linux distributions. If you use another graphical desktop environment, replace @command{eog} with any other image viewer.}. Since he has used it before, he knows that once it opens an image, he can use the @key{ENTER} or @key{SPACE} keys on the keyboard to go to the next image in the directory or the @key{Backspace} key to to go the previous image. So he opens the image of the first object with the command below and with his cup of coffee in his other hand, he flips through his targets very fast to get a good initial impression of the morphologies of these extra Galactic nebulae. @example $ eog 1_crop.jpg @end example @cindex GNU Bash @cindex GNU Emacs @cindex Spiral galaxies @cindex Elliptical galaxies Hubble's cup of coffee is now finished and he also got a nice general impression of the shapes of the nebulae. He tentatively/mentally classified the objects into three classes while doing the visual inspection. One group of the nebulae have a very simple elliptical shape and seem to have no internal special structure, so he gives them code 1. Another clearly different class are those which have spiral arms which he associates with code 2 and finally there seems to be a class of nebulae in between which appear to have a disk but no spiral arms, he gives them code 3. Now he wants to know how many of the nebulae in his extra Galactic sample are within each class. Repeating the same process above and writing the results on paper is very time consuming and prone to errors. Fortunately Hubble knows the basics of GNU Bash shell programming, so he writes the following short script with a loop to help him with the job. After all, computers are made for us to operate and knowing basic shell programming gives Hubble this ability to creatively operate the computer as he wants. So using GNU Emacs@footnote{This can be done with any text editor} (his favorite text editor) he puts the following text in a file named @file{classify.sh}. @example for name in *.jpg do eog $name & processid=$! echo -n "$name belongs to class: " read class echo $name $class >> classified.txt kill $processid done @end example @cindex Gedit @cindex GNU Emacs Fortunately GNU Emacs or even simpler editors like Gedit (part of the GNOME graphical user interface) will display the variables and shell constructs in different colors which can really help in understanding the script. Put simply, the @code{for} loop gets the name of each JPEG file in the directory this script is run in and puts it in @code{name}. In the shell, the value of a variable is used by putting a @code{$} sign before the variable name. Then Eye of GNOME is run on the image in the background to show him that image and its process ID is saved internally (this is necessary to close Eye of GNOME later). The shell then prompts the user to specify a class and after saving it in @code{class}, it prints the file name and the given class in the next line of a file named @file{classified.txt}. To make the script executable (so he can run it later any time he wants) he runs: @example $ chmod +x classify.sh @end example @noindent Now he is ready to do the classification, so he runs the script: @example $ ./classify.sh @end example @noindent In the end he can delete all the JPEG and FITS files along with ImageCrop's log file with the following short command. The only files remaining are the script and the result of the classification. @example $ rm *.jpg *.fits astimgcrop.txt $ ls classified.txt classify.sh @end example @noindent He can now use @file{classified.txt} as input to a plotting program to plot the histogram of the classes and start making interpretations about what these nebulous objects that are outside of the Galaxy are. @node Sufi simulates a detection, , Hubble visually checks and classifies his catalog, Tutorials @section Sufi simulates a detection It is the year 953 A.D. and Sufi@footnote{Abd al-rahman Sufi (903 -- 986 A.D.), also known in Latin as Azophi was an Iranian astronomer. His manuscript ``Book of fixed stars'' contains the first recorded observations of the Andromeda galaxy, the Large Magellanic Cloud and seven other non-stellar or `nebulous' objects.} is in Shiraz as a guest astronomer. He had come there to use the advanced 123 centimeter astrolabe for his studies on the Ecliptic. However, something was bothering him for a long time. While mapping the constellations, there were several non-stellar objects that he had detected in the sky, one of them was in the Andromeda constellation. During a trip he had to Yemen, Sufi had seen another such object in the southern skies looking over the Indian ocean. He wasn't sure if such cloud-like non-stellar objects (which he was the first to call `Sah@={a}bi' in Arabic or `nebulous') were real astronomical objects or if they were only the result of some bias in his observations. Could such diffuse objects actually be detected at all with his detection technique? He still had a few hours left until nightfall (when he would continue his studies on the ecliptic) so he decided to find an answer to this question. He had thoroughly studied Claudius Ptolemy's (90 -- 168 A.D) Almagest and had made lots of corrections to it, in particular in measuring the brightness. Using his same experience, he was able to measure a magnitude for the objects and wanted to simulate his observation to see if a simulated object with the same brightness and size could be detected in a simulated noise with the same detection technique. The general outline of the steps he wants to take are: @enumerate @item Make some mock profiles in an oversampled image. The initial mock image has to be oversampled prior to convolution or other forms of transformation in the image. Through his experiences, Sufi knew that this is because the image of heavenly bodies is actually transformed by the atmosphere or other sources outside the atmosphere (for example gravitational lenses) prior to being sampled on an image. Since that transformation occurs on a continuous grid, to best approximate it, he should do all the work on a finer pixel grid. In the end he can re-sample the result to the initially desired grid size. @item Convolve the image with a PSF image that is oversampled to the same value as the mock image. Since he wants to finish in a reasonable time and the PSF kernel will be very large due to oversampling, he has to use frequency domain convolution which has the side effect of dimming the edges of the image. So in the first step above he also has to build the image to be larger by at least half the width of the PSF convolution kernel on each edge. @item With all the transformations complete, the image should be re-sampled to the same size of the pixels in his detector. @item He should remove those extra pixels on all edges to remove frequency domain convolution artifacts in the final product. @item He should add noise to the (until now, noise-less) mock image. After all, all observations have noise associated with them. @end enumerate Fortunately Sufi had heard of GNU Astronomy Utilities from a colleague in Isfahan (where he worked) and had installed it on his computer a year before. It had tools to do all the steps above. He had used MakeProfiles before, but wasn't sure which columns he had chosen in his user or system wide configuration files for which parameters, see @ref{Configuration files}. So to start his simulation, Sufi runs MakeProfiles with the @option{-P} option to make sure what columns in a catalog MakeProfiles currently recognizes and the output image parameters: @example $ astmkprof -P # MakeProfiles (GNU Astronomy Utilities 0.1) 0.1 # Configured on 21 September 952 at 19:37 # Written on Sat Oct 6 15:49:31 953 # Output: naxis1 1000 naxis2 1000 oversample 5 [[[ Truncated middle of list ]]] # Catalog: xcol 1 ycol 2 fcol 3 rcol 4 ncol 5 pcol 6 qcol 7 mcol 8 tcol 9 [[[ Truncated rest of list ]]] @end example @noindent In particular, Sufi looks at the parameters under the catalog grouping. Fortunately the columns are naturally numbered such that column 0 can be an ID he specifies for each object (which MakeProfiles ignores) and each subsequent column specifies a given parameter. Fortunately MakeProfiles has the capability to also make the PSF which is to be used on the mock image and using the @option{--prepforconv} option, he can also make the mock image to be larger by the correct amount and all the sources to be shifted by the correct amount. For his initial check he decides to simulate the nebula in the Andromeda constellation. The night he was observing, the PSF had roughly a FWHM of about 5 pixels, so as the first row, he defines the PSF parameters and sets the radius column (@code{rcol} above, fifth column) to @code{5.000}, he also chooses a Moffat function for its functional form. Remembering how diffuse the nebula in the Andromeda constellation was, he decides to simulate it with a mock S@'{e}rsic index 1.0 profile. He wants the output to be 500 pixels by 500 pixels, so he puts the mock profile in the center. Looking at his drawings of it, he decides a reasonable effective radius for it would be 40 pixels on this image pixel scale, he sets the axis ratio and position angle to approximately correct values too and finally he sets the total magnitude of the profile to 3.44 which he had accurately measured. Sufi also decides to truncate both the mock profile and PSF at 5 times the respective radius parameters. In the end he decides to put four stars on the four corners of the image at very low magnitudes as a visual scale. Using all the information above, he creates the catalog of mock profiles he wants in a file named @file{cat.txt} (short for catalog) using his favorite text editor and stores it in a directory named @file{simulationtest} in his home directory. [The @command{cat} command prints the contents of a file, short for concatenation. So please copy-paste the outputs of the command ``@command{cat cat.txt}'' into @file{cat.txt} when the editor opens in the steps above it, note that there are 6 lines]: @example $ mkdir ~/simulationtest $ cd ~/simulationtest $ pwd /home/rahman/simulationtest $ emacs cat.txt $ ls cat.txt $ cat cat.txt 0 0.0000 0.0000 1 5.000 4.765 0.0000 1.000 30.000 5.000 1 250.00 250.00 0 40.00 1.000 -25.00 0.400 3.4400 5.000 2 50.000 50.000 3 0.000 0.000 0.0000 0.000 9.0000 0.000 3 450.00 50.000 3 0.000 0.000 0.0000 0.000 9.2500 0.000 4 50.000 450.00 3 0.000 0.000 0.0000 0.000 9.5000 0.000 5 450.00 450.00 3 0.000 0.000 0.0000 0.000 9.7500 0.000 @end example @noindent The zero-point magnitude for his observation was 18. Now he has all the necessary parameters and runs MakeProfiles with the following command: @example $ astmkprof --prepforconv --naxis1=500 --naxis2=500 \ --zeropoint=18.0 cat.txt MakeProfiles started on Sat Oct 6 16:26:56 953 - 6 profiles read from cat.txt in 0.000209 seconds ---- Row 5 complete, 5 left to go. ---- Row 3 complete, 4 left to go. ---- Row 2 complete, 3 left to go. ---- Row 4 complete, 2 left to go. ---- ./0_cat.fits created. ---- Row 0 complete, 1 left to go. ---- Row 1 complete, 0 left to go. - cat.fits created. in 0.024811 seconds MakeProfiles finished in: 0.236629 (seconds) $ls 0_cat.fits astmkprof.log cat.fits cat.txt @end example @cindex Oversample @noindent The file @file{0.fits} is the PSF Sufi had asked for and @file{cat.fits} is the image containing the 5 objects. The PSF is now available to him as a separate file for the convolution step. While he was preparing the catalog, one of his students came up and was also following the steps. When he opened the image, the student was surprised to see that all the stars are only one pixel and not in the shape of the PSF as we see when we image the sky at night. So Sufi explained to him that the stars will take the shape of the PSF after convolution and this is how they would look if we didn't have an atmosphere or an aperture when we took the image. The size of the image was also surprising for the student, instead of 500 by 500, it was 2630 by 2630 pixels. So Sufi had to explain why oversampling is very important for parts of the image where the flux change is significant over a pixel. Sufi then explained to him that after convolving we will re-sample the image to get our originally desired size. To convolve the image, Sufi ran the following command: @example $ astconvolve --kernel=0_cat.fits cat.fits Convolve started on Mon Apr 6 16:35:32 953 Convolving cat.fits (hdu: 0) with the kernel 0.fits (hdu: 0). using 8 CPU threads in the frequency domain. - Input and Kernel images padded. in 0.045576 seconds - Images converted to frequency domain. in 10.486712 seconds - Multiplied in the frequency domain. in 0.032780 seconds - Converted back to the spatial domain. in 5.342335 seconds - Padded parts removed. in 0.011880 seconds Convolve finished in: 15.972771 (seconds) $ls 0_cat.fits astmkprof.log cat_convolved.fits cat.fits cat.txt @end example @noindent When convolution finished, Sufi opened the @file{cat_convolved.fits} file and showed the effect of convolution to his student and explained to him how a PSF with a larger FWHM would make the points even wider. With the convolved image ready, they were ready to re-sample it to the original pixel scale Sufi had planned. Sufi explained the basic concepts of warping the image to his student and ran ImageWarp with the following command: @example $ astimgwarp cat_convolved.fits --scale=0.2 ImageWarp started on Mon Apr 6 16:51:59 953 Using 8 CPU threads. Input image: cat_convolved.fits matrix: 0.2000 0.0000 0.4000 0.0000 0.2000 0.4000 0.0000 0.0000 1.0000 ImageWarp finished in: 0.481421 (seconds) $ ls 0_cat.fits cat_convolved.fits cat.fits astmkprof.log cat_convolved_warped.fits cat.txt @end example @noindent @file{cat_convolved_warped.fits} now has the correct pixel scale. However, the image is still larger than what we had wanted, it is 526 (@mymath{500+13+13}) by 526 pixels. The student is slightly confused, so Sufi also resamples the PSF with ImageWarp and the same warping matrix and shows him that it is 27 (@mymath{2\times13+1}) by 27 pixels. Sufi goes on to explain how frequency space convolution will dim the edges and that is why he added the @option{--prepforconv} option to MakeProfiles, see @ref{If convolving afterwards}. Now that convolution is done Sufi can remove those extra pixels using ImageCrop: @example $ astimgcrop cat_convolved_warped.fits --section=13:*-13,13:*-13 \ --zeroisnotblank ImageCrop started on Sat Oct 6 17:03:24 953 - Read metadata of 1 images. in 0.000560 seconds ---- cat_convolved_warped_crop.fits 1 1 ImageCrop finished in: 0.018917 (seconds) $ls 0_cat.fits astmkprof.log cat_convolved_warped.fits 0_warped.fits cat_convolved.fits cat.fits astimgcrop.log cat_convolved_warped_crop.fits cat.txt @end example @noindent Finally, the @file{cat_convolved_warped.fits} has the same dimensions as Sufi had asked for in the beginning. All this trouble was certainly worth it because now there is no dimming on the edges of the image and the profile centers are more accurately sampled. The final step to simulate a real observation would be to add noise to the image. Sufi set the zeropoint magnitude to the same value that he set when making the mock profiles and looking again at his observation log, he found that at that night the background flux near the nebula had a magnitude of 7. So using these values he ran MakeNoise: @example $ astmknoise --zeropoint=18 --background=7 --output=out.fits \ cat_convolved_warped_crop.fits MakeNoise started on Mon Apr 6 17:05:06 953 - Generator type: mt19937 - Generator seed: 1428318100 MakeNoise finished in: 0.033491 (seconds) $ls 0_cat.fits cat_convolved.fits cat.txt 0_warped.fits cat_convolved_warped_crop.fits out.fits astimgcrop.log cat_convolved_warped.fits astmkprof.log cat.fits @end example @noindent The @file{out.fits} file now has the noised image of the mock catalog Sufi had asked for. Seeing how the @option{--output} option allows the user to specify the name of the output file, the student was confused and wanted to know why Sufi hadn't used it before? Sufi then explained to him that for intermediate steps it is best to rely on the automatic output, see @ref{Automatic output}. Doing so will give all the intermediate files the same basic name structure, so in the end you can simply remove them all with the Shell's capabilities. So Sufi decided to show this to the student by making a shell script from the commands he had used before. The command-line shell has the capability to read all the separate input commands from a file. This is very useful when you want to do the same thing multiple times, with only the names of the files or minor parameters changing between the different instances. Using the shell's history (by pressing the up keyboard key) Sufi reviewed all the commands and then he retrieved the last 5 commands with the @command{$ history 5} command. He selected all those lines he had input and put them in a text file named @file{mymock.sh}. Then he used some shell variables to set the two main constant parts of all the command to generalized variables. @example edge=13 base=cat rm out.fits astmkprof --prepforconv --naxis1=500 --naxis2=500 \ --zeropoint=18.0 "$base".txt astconvolve --kernel=0.fits "$base".fits astimgwarp "$base"_convolved.fits --scale=0.2 astimgcrop "$base"_convolved_warped.fits \ --section=$edge:*-$edge,$edge:*-$edge astmknoise --zeropoint=18 --background=7 --output=out.fits \ "$base"_convolved_warped_crop.fits rm 0*.fits cat*.fits *.log @end example @cindex Gedit @cindex GNU Emacs Sufi then explained to the eager student that you define a variable by giving it a name, followed by an @code{=} sign and the value you want. Then you can reference that variable from anywhere in the script by calling its name with a @code{$} prefix. So in the script whenever you see @code{$base}, the value we defined for it above is used. If you use advanced editors like GNU Emacs or even simpler ones like Gedit (part of the GNOME graphical user interface) the variables will become a different color which can really help in understanding the script. We have put all the @code{$base} variables in double quotation marks (@code{"}) so the variable name and the following text do not get mixed, the shell is going to ignore the @code{"} after replacing the variable value. To make the script executable, Sufi ran the following command: @example $ chmod +x mymock.sh @end example @noindent Then finally, Sufi ran the script, simply by calling its file name: @example $ ./mymock.sh @end example After the script finished, the only file remaining is the @file{out.fits} file that Sufi had wanted in the beginning. Sufi then explained to the student how he could run this script anywhere that he has a catalog if the script is in the same directory. The only thing the student had to modify in the script was the name of the catalog (the value of the @code{base} variable in the start of the script) and the value to the @code{edge} variable if he changed the PSF size. The student was also very happy to hear that he won't need to make it executable again when he makes changes later, it will remain executable unless he explicitly changes the executable flag with @command{chmod}. The student was really excited, since now, through simple shell scripting, he could really speed up his work and run any command in any fashion he likes allowing him to be much more creative in his works. Until now he was using the graphical user interface which doesn't have such a facility and doing repetitive things on it was really frustrating and some times he would make mistakes. So he left to go and try scripting on his own computer. Sufi could now get back to his own work and see if the simulated nebula which resembled the one in the Andromeda constellation could be detected or not. Although it was extremely faint@footnote{The brightness of a diffuse object is added over all its pixels to give its final magnitude, see @ref{Flux Brightness and magnitude}. So although the magnitude 3.44 (of the mock nebula) is orders of magnitude brighter than 6 (of the stars), the central galaxy is much fainter. Put another way, the brightness is distributed over a large area in the case of a nebula.}, fortunately it passed his detection tests and he wrote it in the draft manuscript that would later become ``Book of fixed stars''. He still had to check the other nebula he saw from Yemen and several other such objects, but they could wait until tomorrow (thanks to the shell script, he only has to define a new catalog). It was nearly sunset and they had to begin preparing for the night's measurements on the ecliptic. @node Installation, Common program behavior, Tutorials, Top @chapter Installation @cindex Installation To successfully install and thus use Gnuastro, first please make sure you have the dependencies installed (see @ref{Dependencies}). Only the first group are required when you are building Gnuastro using a tarball (see @ref{Release tarball}), they are very basic and low-level tools used in most astronomical software, so you might already have them installed, if not they are very easy to install as described for each. @ref{Downloading the source} discusses the two methods you can obtain the source code: as a tarball (a significant snapshot in Gnuastro's history), or the full history. The building and installation of Gnuastro is heavily customizable, to learn more about them, see @ref{Build and install}. This section is essentially a thorough explanation of the steps in @ref{Quick start}. It discusses ways you can influence the building and installation. If you encounter any problems in the installation process, it is probably already explained in @ref{Known issues}. In @ref{Other useful software} the installation and usage of some other free software that are not directly required by Gnuastro but might be useful in conjunction with it is discussed. @menu * Dependencies:: Necessary packages for Gnuastro. * Downloading the source:: Ways to download the source code. * Build and install:: Configure, build and install Gnuastro. @end menu @node Dependencies, Downloading the source, Installation, Installation @section Dependencies The dependencies needed to build and install Gnuastro are defined by the features you want and how you would like to obtain the source code (see @ref{Downloading the source}). A minimal set of dependencies are mandatory, if they are not present you cannot get passed the configuration step. Such mandatory dependencies are therefore very basic (low-level) tools which are easy to obtain, build and install, see @ref{Mandatory dependencies} for a full discussion. If you have the packages of @ref{Optional dependencies}, Gnuastro will have additional functionality (for example converting FITS images to JPEG or PDF). If you are installing from a tarball as explained in @ref{Quick start}, you can stop reading after this section. However, if you decided to use the version controlled source instead of the tarball (see @ref{Version controlled source}), an additional bootstrapping step is required before configuration and its dependencies are explained in @ref{Bootstrapping dependencies}. @menu * Mandatory dependencies:: Gnuastro will not install without these. * Optional dependencies:: Adding more functionality. * Bootstrapping dependencies:: If you have the version controlled source. @end menu @node Mandatory dependencies, Optional dependencies, Dependencies, Dependencies @subsection Mandatory dependencies @cindex Dependencies, Gnuastro @cindex GNU build system The mandatory Gnuastro dependencies are very basic and low-level tools. They all follow the same basic GNU based build system (like that shown in @ref{Quick start}), so even if you don't have them, installing them should be pretty straightforward. In this section we explain each program and any specific note that might be necessary in the installation. @cindex Building from source @cindex Compiling from source @cindex Source code building @cindex Source code compilation @cindex Package managers The most basic choice is to build the packages from source yourself, instead of relying on your distribution's package management system. While the latter choice is indeed possible, we recommend that you build these dependencies yourself as discussed below. We will send out notifications in the @command{info-gnuastro} mailing list, see @ref{Announcements} when we find out that these requirements are updated. @enumerate @item For each package, Gnuastro might preform better (or require) certain configuration options that your distribution's package managers didn't add for you. If present, these configuration options are explained during the installation of each in the sections below. When the proper configuration has not been set, the programs should complain and inform you. @item Your distribution's pre-built package might not be the most recent release. @item For the libraries, they might separate the binary file from the header files, see @ref{Known issues}. @item Like any other tool, the science you derive from Gnuastro's tools highly depend on these lower level dependencies, so generally it is much better to have a close connection with them. By reading their manuals, installing them and staying up to date with changes/bugs in them, your scientific results and understanding will also correspondingly improve. @end enumerate @menu * GNU Scientific Library:: Installing GSL. * CFITSIO:: C interface to the FITS standard. * WCSLIB:: C interface to the WCS standard of FITS. @end menu @node GNU Scientific Library, CFITSIO, Mandatory dependencies, Mandatory dependencies @subsubsection GNU Scientific library @cindex GNU Scientific Library The @url{http://www.gnu.org/software/gsl/, GNU Scientific Library}, or GSL, is a large collection of functions that are very useful in scientific applications, for example integration, random number generation, and Fast Fourier Transform among many others. To install GSL from source, you can run the following commands after you have downloaded @url{ftp://ftp.gnu.org/gnu/gsl/gsl-latest.tar.gz, @file{gsl-latest.tar.gz}}: @example $ tar xf gsl-latest.tar.gz $ cd gsl-X.X # Replace X.X with version number $ ./configure $ make $ make check $ sudo make install @end example @node CFITSIO, WCSLIB, GNU Scientific Library, Mandatory dependencies @subsubsection CFITSIO @cindex CFITSIO @cindex FITS standard @url{http://heasarc.gsfc.nasa.gov/fitsio/, CFITSIO} is the closest you can get to the pixels in a FITS image while remaining faithful to the @url{http://fits.gsfc.nasa.gov/fits_standard.html, FITS standard}. It is written by William Pence, the principal author of the FITS standard@footnote{Pence, W.D. et al. Definition of the Flexible Image Transport System (FITS), version 3.0. (2010) Astronomy and Astrophysics, Volume 524, id.A42, 40 pp.}, and is regularly updated. Setting the definitions for all other software packages using FITS images. @vindex --enable-reentrant @cindex Reentrancy, multiple file opening @cindex Multiple file opening, reentrancy Some GNU/Linux distributions have CFITSIO in their package managers, if it is available and updated, you can use it. One problem that might occur is that CFITSIO might not be configured with the @option{--enable-reentrant} option by the distribution. This option allows CFITSIO to open a file in multiple threads, it can thus provide great speed improvements. If CFITSIO was not configured with this option, any program which needs this capability will warn you and abort when you ask for multiple threads (see @ref{Threads in Gnuastro}). To install CFITSIO from source, we strongly recommend that you have a look through Chapter 2 (Creating the CFITSIO library) of the CFITSIO manual and understand the options you can pass to @command{$ ./configure} (they aren't too much). This is a very basic package for most astronomical software and it is best that you configure it nicely with your system. Once you download the source and unpack it, the following configure script should be enough for most purposes. Don't forget to read chapter two of the manual though, for example the second option is only for 64bit systems. The manual also explains how to check if it has been installed correctly. CFITSIO comes with two executables called fpack and funpack. From their manual: they ``are standalone programs for compressing and uncompressing images and tables that are stored in the FITS (Flexible Image Transport System) data format. They are analogous to the gzip and gunzip compression programs except that they are optimized for the types of astronomical images that are often stored in FITS format''. The instruction below explain how to compile and install them on your system along with CFITSIO. They are not essential for Gnuastro, since they are just wrappers for functions within CFITSIO, but they can come in handy. The @command{make utils} command is only available for versions above 3.39, it will build these executables along with several other test executables which are deleted before the installation (otherwise they will also be installed). The CFITSIO installation from source process is given below. Let's assume you have downloaded @url{http://heasarc.gsfc.nasa.gov/FTP/software/fitsio/c/cfitsio_latest.tar.gz, @file{cfitsio_latest.tar.gz}} and are in the same directory: @example $ tar xf cfitsio_latest.tar.gz $ cd cfitsio $ ./configure --prefix=/usr/local --enable-sse2 --enable-reentrant $ make $ make utils $ ./testprog > testprog.lis $ diff testprog.lis testprog.out # Should have no output $ cmp testprog.fit testprog.std # Should have no output $ rm cookbook fitscopy imcopy smem speed testprog $ sudo make install @end example @node WCSLIB, , CFITSIO, Mandatory dependencies @subsubsection WCSLIB @cindex WCS @cindex WCSLIB @cindex World Coordinate System @url{http://www.atnf.csiro.au/people/mcalabre/WCS/, WCSLIB} is written and maintained by one of the authors of the World Coordinate System (WCS) definition in the @url{http://fits.gsfc.nasa.gov/fits_standard.html, FITS standard}@footnote{Greisen E.W., Calabretta M.R. (2002) Representation of world coordinates in FITS. Astronomy and Astrophysics, 395, 1061-1075.}, Mark Calabretta. It might be already built and ready in your distribution's package management system. However, here the installation from source is explained, for the advantages please see @ref{Mandatory dependencies}. To install WCSLIB you will need to have CFITSIO already installed, see @ref{CFITSIO}. @vindex --without-pgplot WCSLIB also has plotting capabilities which use PGPLOT (a plotting library for C). If you wan to use those capabilities in WCSLIB, @ref{PGPLOT} provides the PGPLOT installation instructions. However PGPLOT is old@footnote{As of early June 2016, its most recent version was uploaded in February 2001.}, so its installation is not easy, there are also many great modern WCS plotting tools (mostly in written in Python). Hence, if you will not be using those plotting functions in WCSLIB, you can configure it with the @option{--without-pgplot} option as shown below. Let's assume you have downloaded @url{ftp://ftp.atnf.csiro.au/pub/software/wcslib/wcslib.tar.bz2, @file{wcslib.tar.bz2}} and are in the same directory: @example $ tar xf wcslib.tar.bz2 $ cd wcslib-X.X # Replace X.X with version number $ ./configure --without-pgplot LIBS="-pthread -lm" $ make $ make check $ sudo make install @end example @node Optional dependencies, Bootstrapping dependencies, Mandatory dependencies, Dependencies @subsection Optional dependencies The libraries listed here are only used for very specific applications, therefore if you don't want these operations, Gnuastro will be built and installed without them and you don't have to have the dependencies. @cindex GPL Ghostscript If the @command{./configure} script can't find these requirements, it will warn you in the end that they are not present and notify you of the operation(s) you can't do due to not having them. If the output you request from a program requires a missing library, that program is going to warn you and abort. In the case of executables like GPL GhostScript, if you install them at a later time, the program will run. This is because if required libraries are not present at build time, the executables cannot be built, but an executable is called by the built program at run time so if it becomes available, it will be used. If you do install an optional library later, you will have to rebuild Gnuastro and reinstall it for it to take effect. @table @asis @item libgit2 @cindex Git @cindex libgit2 @cindex Version control systems Git is one of the most common version control systems (see @ref{Version controlled source}). When @file{libgit2} is present, all Gnuastro's outputs will contain the version number of the working directory's repository for future reproducibility. See the @command{COMMIT} keyword header in @ref{Output headers} for a discussion. @item libjpeg @pindex libjpeg @cindex JPEG format libjpeg is only used by ConvertType to read from and write to JPEG images. @url{http://www.ijg.org/, libjpeg} is a very basic library that provides tools to read and write JPEG images, most of the GNU/Linux graphic programs and libraries use it. Therefore you most probably already have it installed. @url{http://libjpeg-turbo.virtualgl.org/, libjpeg-turbo} is an alternative to libjpeg. It uses SIMD instructions for ARM based systems that significantly decreases the processing time of JPEG compression and decompression algorithms. @item GPL Ghostscript @cindex GPL Ghostscript GPL Ghostscript's executable (@command{gs}) is called used by ConvertType to compile a PDF file from a source PostScript file, see @ref{ConvertType}. Therefore its headers (and libraries) are not needed. With a very high probability you already have it in your GNU/Linux distribution. Unfortunately it does not follow the standard GNU build style so installing it is very hard. It is best to rely on your distribution's package managers for this. @end table @node Bootstrapping dependencies, , Optional dependencies, Dependencies @subsection Bootstrapping dependencies Bootstrapping is only necessary if you have decided to obtain the full version controlled history of Gnuastro, see @ref{Version controlled source} and @ref{Bootstrapping}. Using the version controlled source enables you to always be up to date with the most recent development work of Gnuastro (bug fixes, new functionalities, improved algorithms and etc). If you have downloaded a tarball (see @ref{Downloading the source}), then you can ignore this subsection. To successfully run the bootstrapping process, there are some additional dependencies to those discussed in the previous subsections. These are low level tools that are used by a large collection of Unix-like operating systems programs, therefore they are most probably already available in your system. If they are not already installed, you should be able to easily find them in any GNU/Linux distribution package management system (@command{apt-get}, @command{yum}, @command{pacman} and etc). The short names in parenthesis in @command{typewriter} font after the package name can be used to search for them in your package manager. For the GNU Portability Library, GNU Autoconf Archive and @TeX{} Live, it is recommended to use the instructions here, not your operating system's package manager. @table @asis @item GNU Portability Library (Gnulib) @cindex GNU C library @cindex Gnulib: GNU Portability Library @cindex GNU Portability Library (Gnulib) To ensure portability for a wider range of operating systems (those that don't include GNU C library, namely glibc), Gnuastro depends on the GNU portability library, or Gnulib. Gnulib keeps a copy of all the functions in glibc, implemented (as much as possible) to be portable to other operating systems. The @file{bootstrap} script can automatically clone Gnulib (as a @file{gnulib/} directory inside Gnuastro), however, as described in @ref{Bootstrapping} this is not recommended. The recommended way to bootstrap Gnuastro is to first clone Gnulib and the Autoconf archives (see below) into a local directory outside of Gnuastro. Let's call it @file{DEVDIR}@footnote{If you are not a developer in Gnulib or Autoconf archives, @file{DEVDIR} can be a directory that you don't backup. In this way the large number of files in these projects won't slow down your backup process or take bandwidth (if you backup to a remote server).} (which you can set to any directory). Currently in Gnuastro, both Gnulib and Autoconf archives have to be cloned in the same top directory@footnote{If you already have the Autoconf archives in a separate directory, or can't clone it in the same directory as Gnulib, or you have it with another directory name (not @file{autoconf-archive/}), you can follow this short step. Set @file{AUTOCONFARCHIVES} to your desired address. Then define a symbolic link in @file{DEVDIR} with the following command so Gnuastro's bootstrap script can find it:@*@command{$ ln -s $AUTOCONFARCHIVES $DEVDIR/autoconf-archive}.} like the case here@footnote{If your internet connection is active, but Git complains about the network, it might be due to your network setup not recognizing the git protocol. In that case use the following URL for the HTTP protocol instead (for Autoconf archives, replace the name): @command{http://git.sv.gnu.org/r/gnulib.git}}: @example $ DEVDIR=/home/yourname/Development $ cd $DEVDIR $ git clone git://git.sv.gnu.org/gnulib.git $ git clone git://git.sv.gnu.org/autoconf-archive.git @end example @noindent You now have the full version controlled source of these two repositories in separate directories. Both these packages are regularly updated, so every once in a while, you can run @command{$ git pull} within them to get any possible updates. @item GNU Automake (@command{automake}) @cindex GNU Automake GNU Automake will build the @file{Makefile.in} files in each sub-directory using the (hand-written) @file{Makefile.am} files. The @file{Makefile.in}s are subsequently used to generate the @file{Makefile}s when the user runs @command{./configure} before building. @item GNU Autoconf (@command{autoconf}) @cindex GNU Autoconf GNU Autoconf will build the @file{configure} script using the configurations we have defined (hand-written) in @file{configure.ac}. @item GNU Autoconf Archive @cindex GNU Autoconf Archive These are a large collection of tests that can be called to run at @command{./configure} time. See the explanation under GNU Portability Library above for instructions on obtaining it and keeping it up to date. @item GNU Libtool (@command{libtool}) @cindex GNU Libtool GNU Libtool is in charge of building all the libraries in Gnuastro. The libraries contain functions that are used by more than one program and are installed for use in other programs. They are thus put in a separate directory (@file{lib/}). @item GNU help2man (@command{help2man}) @cindex GNU help2man GNU help2man is used to convert the output of the @option{--help} option (@ref{--help}) to the traditional Man page (@ref{Man pages}). @item @LaTeX{} and some @TeX{} packages @cindex @LaTeX{} @cindex @TeX{} Live Some of the figures in this book are built by @LaTeX{} (using the PGF/TikZ package). The @LaTeX{} source for those figures is version controlled for easy maintenance not the actual figures. So the @file{./boostrap} script will run @LaTeX{} to build the figures. The best way to install @LaTeX{} and all the necessary packages is through @url{https://www.tug.org/texlive/, @TeX{} live} which is a package manager for @TeX{} related tools that is independent of any operating system. It is thus preferred to the @TeX{} Live versions distributed by your operating system. To install @TeX{} Live, go to the webpage and download the appropriate installer by following the ``download'' link. Note that by default the full package repository will be downloaded and installed (around 4 Giga Bytes) which can take @emph{very} long to download and to update later. However, most packages are not needed by everyone, it is easier, faster and better to install only the ``Basic scheme'' (consisting of only the most basic @TeX{} and @LaTeX{} packages, which is less than 200 Mega bytes)@footnote{You can also download the DVD iso file at a later time to keep as a backup for when you don't have internet connection if you need a package.}. After the installation be sure to set the environment variables as suggested in the end of the outputs. Any time you confront (need) a package you don't have, simply install it with a command like below (similar to how you install software from your operating system's package manager)@footnote{After running @TeX{}, or @LaTeX{}, you might get a warning complaining about a @file{missingfile}. Run `@command{tlmgr info missingfile}' to see the package(s) containing that file which you can install.}. To install all the necessary @TeX{} packages for a successful Gnuastro bootstrap, run this command: @example $ su # tlmgr install epsf jknapltx caption biblatex biber iftex \ etoolbox logreq xstring xkeyval pgf ms \ xcolor pgfplots times rsfs pstools epspdf @end example @item ImageMagick (@command{imagemagick}) @cindex ImageMagick ImageMagick is a wonderful and robust program for image manipulation on the command-line. @file{bootsrap} uses it to convert the book images into the formats necessary for the various book formats. @end table @node Downloading the source, Build and install, Dependencies, Installation @section Downloading the source Gnuastro's source code can be downloaded in two ways. As a tarball, ready to be configured and installed on your system (as described in @ref{Quick start}), see @ref{Release tarball}. If you want official releases of stable versions this is the best, easiest and most common option. Alternatively, you can clone the version controlled history of Gnuastro, run one extra bootstrapping step and then follow the same steps as the tarball. This will give you access to all the most recent work that will be included in the next release along with the full project history. The process is thoroughly introduced in @ref{Version controlled source}. @menu * Release tarball:: Download a stable official release. * Version controlled source:: Get and use the version controlled source. @end menu @node Release tarball, Version controlled source, Downloading the source, Downloading the source @subsection Release tarball A release tarball (commonly compressed) is the most common way of obtaining free and open source software. A tarball is a snapshot of one particular moment in the Gnuastro development history along with all the necessary files to configure, build, and install Gnuastro easily (see @ref{Quick start}). It is very straightforward and needs the least set of dependencies (see @ref{Mandatory dependencies}). Gnuastro has tarballs for official stable releases and pre-releases for testing. See @ref{Version numbering} for more on the two types of releases and the formats of the version numbers. The URLs for each type of release are given below. @table @asis @item Official stable releases (@url{http://ftp.gnu.org/gnu/gnuastro}): This URL hosts the official stable releases of Gnuastro. Always use the most recent version (see @ref{Version numbering}). By clicking on the ``Last modified'' title of the second column, the files will be sorted by their date which you can also use to find the latest version. It is recommended to use a mirror to download these tarballs, please visit @url{http://ftpmirror.gnu.org/gnuastro/} and see below. @item Pre-release tar-balls (@url{http://alpha.gnu.org/gnu/gnuastro}): This URL contains unofficial pre-release versions of Gnuastro. The pre-release versions of Gnuastro here are for enthusiasts to try out before an official release. If there are problems, or bugs then the testers will inform the developers to fix before the next official release. See @ref{Version numbering} to understand how the version numbers here are formatted. If you want to remain even more up-to-date with the developing activities, please clone the version controlled source as described in @ref{Version controlled source}. @end table @cindex Gzip @cindex Lzip Gnuastro's official tarball is released with two formats: Gzip (with suffix @file{.tar.gz}) and Lzip (with suffix @file{.tar.lz}). The former is a very well-known and widely used compression program created by GNU and available in most systems. The latter provides a better compression ratio and more robust archival capacity. For example Gnuastro 0.2's tarball was 2.8MB and 4.2MB with Lzip and Gzip respectively. From the @url{http://www.nongnu.org/lzip/lzip.html, Lzip webpage}: ``Lzip is a lossless data compressor with a user interface similar to the one of gzip or bzip2. Lzip can compress about as fast as gzip (@command{lzip -0}), or compress most files more than bzip2 (@command{lzip -9}). Decompression speed is intermediate between gzip and bzip2. Lzip is better than gzip and bzip2 from a data recovery perspective.'' However, Lzip is currently not too common, so it might not be pre-installed in your operating system. Installing it from your operating system's package manager or from source is very easy. The GNU FTP server is mirrored (has backups) in various locations on the globe (@url{http://www.gnu.org/order/ftp.html}). You can use the closest mirror to your location for a more faster download. Note that only some mirrors keep track of the pre-release (alpha) tarballs. Also note that if you want to download immediately after and announcement (see @ref{Announcements}), the mirrors might need some time to synchronize with the main GNU FTP server. @node Version controlled source, , Release tarball, Downloading the source @subsection Version controlled source @cindex Git @cindex Version control The publicly distributed Gnuastro tar-ball (for example @file{gnuastro-X.X.tar.gz}) does not contain the revision history, it is only a snapshot of the source code at one significant instant of Gnuastro's history (specified by the version number, see @ref{Version numbering}), ready to be configured and built. To be able to develop successfully, the revision history of the code can be very useful to track when something was added or changed, also some updates that are not yet officially released might be in it. We use Git for the version control of Gnuastro. For those who are not familiar with it, we recommend the Pro Git@footnote{@url{https://progit.org/}} book. The whole book is publicly available for online reading and downloading and does a wonderful job at explaining the concepts and best practices. Let's assume you want to keep Gnuastro in the @file{TOPGNUASTRO} directory (can be any directory, change the value below). The full version controlled history of Gnuastro can be cloned in @file{TOPGNUASTRO/gnuastro} by running the following commands@footnote{If your internet connection is active, but Git complains about the network, it might be due to your network setup not recognizing the Git protocol. In that case use the following URL which uses the HTTP protocol instead: @command{http://git.sv.gnu.org/r/gnuastro.git}}: @example $ TOPGNUASTRO=/home/yourname/Research/projects/ $ cd $TOPGNUASTRO $ git clone git://git.sv.gnu.org/gnuastro.git @end example @noindent The @file{$TOPGNUASTRO/gnuastro} directory will contain hand-written (version controlled) source code for Gnuastro's programs, libraries, this book and the tests. All are divided into sub-directories with standard and very descriptive names. The version controlled files in the top cloned directory are either mainly in capital letters (for example @file{THANKS} and @file{README}) or mainly written in small-caps (for example @file{configure.ac} and @file{Makefile.am}). The former are non-programming, standard writing for human readers containing high-level information about the whole package. The latter are instructions to customize the GNU build system for Gnuastro. The cloned Gnuastro source cannot immediately be configured, compiled, or installed since it only contains hand-written files, not automatically generated or imported files which do all the hard work of the build process. See @ref{Bootstrapping} for the process of generating and importing those files (it is very easy!). Once you have bootstrapped Gnuastro, you can run the standard procedures (in @ref{Quick start}). Very soon after you have cloned it, Gnuastro's main @file{master} branch will be updated on the main repository (since the developers are actively working on Gnuastro), for the best practices in keeping your local history in sync with the main repository see @ref{Synchronizing}. @menu * Bootstrapping:: Adding all the automaticly generated files. * Synchronizing:: Keep your local clone up to date. @end menu @node Bootstrapping, Synchronizing, Version controlled source, Version controlled source @subsubsection Bootstrapping @cindex Bootstrapping @cindex GNU Autoconf Archive @cindex Gnulib: GNU Portability Library @cindex GNU Portability Library (Gnulib) @cindex Automatically created build files @noindent The version controlled source code lacks the source files that we have not written or are automatically built. These automatically generated files are included in the distributed tar ball for each distribution (for example @file{gnuastro-X.X.tar.gz}, see @ref{Version numbering}) and make it easy to immediately configure, build, and install Gnuastro. However from the perspective of version control, they are just bloatware and sources of confusion (since they are not changed by Gnuastro developers). The process of automatically building and importing necessary files into the cloned directory is known as @emph{bootstrapping}. All the instructions for an automatic bootstrapping are available in @file{bootstrap} and configured using @file{bootstrap.conf}. @file{bootstrap} is the only file not written by Gnuastro developers but is under version control to enable simple bootstrapping immediately after cloning. It is maintained by the GNU Portability Library (Gnulib) and this file is an identical copy, so do not make any changes in this file since it will be replaced when Gnulib releases an update. Make all your changes in @file{bootstrap.conf}. The bootstrapping process has its own separate set of dependencies, the full list is given in @ref{Bootstrapping dependencies}. They are generally very low-level and used by a very large set of commonly used programs, so they are probably already installed on your system. The simplest way to bootstrap Gnuastro is to simply run the bootstrap script within your cloned Gnuastro directory as shown below. However, please read the next paragraph before doing so (see @ref{Version controlled source} for @file{TOPGNUASTRO}). @example $ cd TOPGNUASTRO/gnuastro $ ./bootstrap # Requires internet connection @end example Without any options, @file{bootstrap} will clone Gnulib within your cloned Gnuastro directory (@file{TOPGNUASTRO/gnuastro/gnulib}) and download the necessary Autoconf archives macros. So if you run bootstrap like this, you will need an internet connection every time you decide to bootstrap. Also, Gnulib is a large package and cloning it can be slow. It will also keep the full Gnulib repository within your Gnuastro repository, so if another one of your projects also needs Gnulib, and you insist on running bootstrap like this, you will have two copies. In case you regularly backup your important files, Gnulib will also slow down the backup process. Therefore while the simple invocation above can be used with no problem, it is not recommended, see the next paragraph. The recommended way to get these two packages is thoroughly discussed in @ref{Bootstrapping dependencies} (in short: clone them in the separate @file{DEVDIR/} directory). The following commands will take you into the cloned Gnuastro directory and run the @file{bootstrap} script, while telling it to copy some files (instead of making symbolic links, with the @option{--copy} option, this is not mandatory@footnote{The @option{--copy} option is recommended because some backup systems might do strange things with symbolic links.}) and where to look for Gnulib (with the @option{--gnulib-srcdir} option). @example $ cd $TOPGNUASTRO/gnuastro $ ./bootstrap --copy --gnulib-srcdir=$DEVDIR/gnulib @end example @cindex GNU Texinfo @cindex GNU Libtool @cindex GNU Autoconf @cindex GNU Automake @cindex GNU C library @cindex GNU build system Since Gnulib and Autoconf archives are now available in your local directories, you don't need an internet connection every time you decide to remove all untracked files and redo the bootstrap (see box below). You can also use the same command on any other project that uses Gnulib. All the necessary GNU C library functions, Autoconf macros and Automake inputs are now available along with the book figures. The standard GNU build system (@ref{Quick start}) will do the rest of the job. @cartouche @noindent @strong{Undoing the bootstrap:} During the development, it might happen that you want to remove all the automatically generated and imported files. In other words, you might want to reverse the bootstrap process. Fortunately Git has a good program for this job: @command{git clean}. Run the following command and every file that is not version controlled will be removed. @example git clean -fxd @end example @noindent It is best to commit any recent change before running this command. You might have created new files since the last commit and if they haven't been committed, they will all be gone forever (using @command{rm}). To get a list of the non-version controlled files instead of deleting them, add the @option{n} option to @command{git clean}, so it becomes @option{-fxdn}. @end cartouche Besides the @file{bootstrap} and @file{bootstrap.conf}, the @file{bootstrapped/} directory and @file{README-hacking} file are also related to the bootstrapping process. The former hosts all the imported (bootstrapped) directories. Thus, in the version controlled source, it only contains a @file{REAME} file, but in the distributed tar-ball it also contains sub-directories filled with all bootstrapped files. @file{README-hacking} contains a summary of the bootstrapping process discussed in this section. It is a necessary reference when you haven't built this book yet. It is thus not distributed in the Gnuastro tarball. @node Synchronizing, , Bootstrapping, Version controlled source @subsubsection Synchronizing The bootstrapping script (see @ref{Bootstrapping}) is not regularly needed: you mainly need it after you have cloned Gnuastro (once) and whenever you want to re-import the files from Gnulib, or Autoconf archives@footnote{@url{https://savannah.gnu.org/task/index.php?13993} is defined for you to check if significant (for Gnuastro) updates are made in these repositories, since the last time you pulled from them.} (not too common). However, Gnuastro developers are constantly working on Gnuastro and are pushing their changes to the official repository. Therefore, your local Gnuastro clone will soon be out-dated. Gnuastro has two mailing lists dedicated to its developing activities (see @ref{Developing mailing lists}). Subscribing to them can help you decide when to synchronize with the official repository. To pull all the most recent work in Gnuastro, run the following command from the top Gnuastro directory: @example $ git pull && autoconf -f @end example @cindex GNU Autoconf @cindex Mailing list: info-gnuastro @cindex @code{info-gnuastro@@gnu.org} GNU Autoconf is part of the GNU build system and will update the @file{./configure} script based on the hand-written configurations (in @file{configure.ac}, which is version controlled in Gnuastro). The pulled changes might contain changes in the build system configurations. However, The most important reason for running this command is to generate a version number for your Gnuastro snapshot. This generated version number will include the commit information if you are building Gnuastro from any point in Gnuastro's history (see @ref{Version numbering}). Since the version number is included in nearly all outputs of the programs, this can help you later exactly reproduce an old result by checking out the exact point in Gnuastro's history that produced those results. Therefore, be sure to run `@file{autoconf -f}' after every synchronization. You can also run them separately: @example $ git pull $ autoconf -f @end example If you would like to see what has changed since you last synchronized your local clone, you can take the following steps instead of the simple command above (don't type anything after @code{#}): @example $ git checkout master # Confirm if you are on master. $ git fetch origin # Fetch all new commits from server. $ git log master..origin/master # See all the new commit messages. $ git merge origin/master # Update your master branch. $ autoconf -f # Update ./configure. @end example @noindent By default @command{git log} prints the most recent commit first, add the @option{--reverse} option to see the changes chronologically. To see exactly what has been changed in the source code along with the commit message, add a @option{-p} option to the @command{git log}. If you intend make changes in the code, have a look at @ref{Developing} to get started easily. Be sure to commit your changes in a separate branch (keep your @code{master} branch to follow the official repository) and re-run @command{autoconf -f} after the commit. If you intend to send your changes to us (see @ref{Contributing to Gnuastro}) for the benefit of the whole community. If you send your work to us, you can safely use your commit since it will be ultimately recorded in Gnuastro's official history. If not, please upload your separate branch to a public hosting service (for example GitLab, see @ref{Forking tutorial}) and link to it in your report, or run @command{make distcheck} and upload the output @file{gnuastro-X.X.X.XXXX.tar.gz} to a publicly accessible webpage so your results can be considered scientific (reproducible). @node Build and install, , Downloading the source, Installation @section Build and install This section is basically a longer explanation to the sequence of commands given in @ref{Quick start}. If you didn't have any problems during the @ref{Quick start} steps, you want to have all the programs of Gnuastro installed in your system, you don't want to change the executable names during or after installation, you have root access to install the programs in the default system wide directory, the Letter paper size of the print book is fine for you or as a summary you don't feel like going into the details when everything is working, you can safely skip this section. If you have any of the above problems or you want to understand the details for a better control over your build and install, read along. The dependencies which you will need prior to configuring, building and installing Gnuastro are explained in @ref{Dependencies}. The first three steps in @ref{Quick start} need no extra explanation, so we will skip them and start with an explanation of Gnuastro specific configuration options and a discussion on the installation directory in @ref{Configuring}, followed by some smaller subsections: @ref{Tests}, @ref{A4 print book}, and @ref{Known issues} which explains the solutions to known problems you might encounter in the installation steps and ways you can solve them. @menu * Configuring:: Configure Gnuastro * Tests:: Run tests to see if it is working. * A4 print book:: Customize the print book. * Known issues:: Issues you might encounter. @end menu @node Configuring, Tests, Build and install, Build and install @subsection Configuring @pindex ./configure @cindex Configuring The @command{$ ./configure} step is the most important step in the build and install process. All the required packages, libraries, headers and environment variables are checked in this step. The behaviors of make and make install can also be set through command line options to this command. @cindex Configure options @cindex Customizing installation @cindex Installation, customizing The configure script accepts various arguments and options which enable the final user to highly customize whatever she is building. The options to configure are generally very similar to normal program options explained in @ref{Arguments and options}. Similar to all GNU programs, you can get a full list of the options along with a short explanation by running @example $ ./configure --help @end example @noindent @cindex GNU Autoconf A complete explanation is also included in the @file{INSTALL} file. Note that this file was written by the authors of GNU Autoconf (which builds the @file{configure} script), therefore it is common for all programs which use the @command{$ ./configure} script for building and installing, not just Gnuastro. Here we only discuss cases where you don't have super-user access to the system and if you want to change the executable names. But before that, a review of the options to configure that are particular to Gnuastro are discussed. @menu * Gnuastro configure options:: Configure options particular to Gnuastro. * Installation directory:: Specify the directory to install. * Executable names:: Changing executable names. * Configure and build in RAM:: For minimal use of HDD or SSD, and clean source. @end menu @node Gnuastro configure options, Installation directory, Configuring, Configuring @subsubsection Gnuastro configure options @cindex @command{./configure} options @cindex Configure options particular to Gnuastro Most of the options to configure (which are to do with building) are similar for every program which uses this script. Here the options that are particular to Gnuastro are discussed. The next topics explain the usage of other configure options which can be applied to any program using the GNU build system (through the configure script). @vtable @option @item --enable-progname Only build and install @file{progname} along with any other program that is enabled in this fashion. @file{progname} is the name of the executable without the @file{ast}, for example @file{imgcrop} for ImageCrop (with the executable name of @file{astimgcrop}). If this option is called for any of the programs in Gnuastro, any program which is not explicitly enabled will not be built or installed. @item --disable-progname @itemx --enable-progname=no Do not build or install the program named @file{progname}. This is very similar to the @option{--enable-progname}, but will build and install all the other programs except this one. @item --enable-gnulibcheck @cindex GNU C library @cindex Gnulib: GNU Portability Library @cindex GNU Portability Library (Gnulib) Enable checks on the GNU Portability Library (Gnulib). Gnulib is used by Gnuastro to enable users of non-GNU based operating systems (that don't use GNU C library or glibc) to compile and use the advanced features that this library provides. We make extensive use of such functions. If you give this option to @command{$ ./configure}, when you run @command{$ make check}, first the functions in Gnulib will be tested, then the Gnuastro executables. If your operating system does not support glibc or has an older version of it and you have problems in the build process (@command{$ make}), you can give this flag to configure to see if the problem is caused by Gnulib not supporting your operating system or Gnuastro, see @ref{Known issues}. @item --disable-guide-message @itemx --enable-guide-message=no Do not print a guiding message during the GNU Build process of @ref{Quick start}. By default, after each step, a message is printed guiding the user what the next command should be. Therefore, after @command{./configure}, it will suggest running @command{make}. After @command{make}, it will suggest running @command{make check} and so on. If Gnuastro is configured with this option, for example @example $ ./configure --disable-guide-message @end example Then these messages will not be printed after any step (like most programs). For people who are not yet fully accustomed to this build system, these guidelines can be very useful and encouraging. However, if you find those messages annoying, use this option. @end vtable @cartouche @noindent @strong{Note:} If some programs are enabled and some are disabled, it is equivalent to simply enabling those that were enabled. Listing the disabled programs is redundant. @end cartouche Note that the tests of some programs might require other programs to have been installed and tested. For example MakeProfiles is the first program to be tested when you run @command{$ make check}, it provides the inputs to all the other tests. So if you don't install MakeProfiles, then the tests for all the other programs will be skipped or fail. To avoid this, in one run, you can install all the packages and run the tests but not install. If everything is working correctly, you can run configure again with only the packages you want but not run the tests and directly install after building. @node Installation directory, Executable names, Gnuastro configure options, Configuring @subsubsection Installation directory @vindex --prefix @cindex Superuser, not possible @cindex Root access, not possible @cindex No access to super-user install @cindex Install with no super-user access One of the most commonly used options to configure is the directory that will host all the files which require installing (for example the actual executable files for the program and/or the documentation and configuration files). This is done through the @option{--prefix} option. To demonstrate its applicability, let's assume you don't have administrator or root access but you want to be able to access the installed files from anywhere while you are logged in (one of the most common uses of @option{--prefix}). The most basic way to run an executable is to explicitly type the full file name (including all the directory information) and run it. One example is running the configuration script with the @command{$ ./configure} command (see @ref{Quick start}). By giving a specific directory (the current directory or @file{./}), we are explicitly telling the shell to look in the current directory for an executable file named `@file{configure}'. Directly specifying the directory is thus useful for simple shell scripts in the current (or nearby) directories. However, when the program (an executable) is to be used a lot, specifying all those directories will become a significant burden. For example, the @file{ls} executable lists the contents in a given directory and it is (usually) installed in the @file{/usr/bin/} directory by the operating system maintainers. So each time you you want to use it you would have to run the following command (which is very inconvenient, both in typing and in remembering the various directories). @example $ /usr/bin/ls @end example @cindex Shell variables @cindex Environment variables To address this problem, we have the @file{PATH} environment variable. To understand it better, we will start with a short introduction to the shell variables. Shell variable values are basically treated as strings of characters. You can define a variable and a value for it by running @example $ myvariable=a_test_value @end example @noindent You can see the value it represents by running @example $ echo $myvariable @end example @noindent @cindex Environment @cindex Environment variables If a variable has no value, the last command will only print an empty line. A variable defined like this will be known as long as this shell or terminal is running. Other terminals will have no idea it existed. The main advantage of shell variables is that if they are exported@footnote{By running @command{$ export myvariable=a_test_value} instead of the simpler case in the text}, subsequent programs that are run within that shell can access their value. So by giving them different values, you can change the ``environment'' of a program which uses their values. The shell variables which are accessed by programs are therefore known as ``environment variables''@footnote{You can use shell variables for other actions too, for example to temporarily keep some names or run loops on some files.}. You can see the full list of the environment variables that your shell currently recognizes by running: @example $ printenv @end example @cindex @file{HOME} @cindex @file{HOME/.local/} @cindex Environment variable, @code{HOME} @file{HOME} is one commonly used environment variable, it is any user's (the one that is logged in) top directory. It is used so often that the shell has a special expansion (alternative) for it: `@file{~}'. Whenever you see file names starting with the tilde sign, it actually represents the value to the @file{HOME} environment variable, so @file{~/doc} is the same as @file{$HOME/doc}. @vindex PATH @pindex ./configure @cindex Setting @code{PATH} @cindex Default executable search directory @cindex Search directory for executables Another one of the most commonly used environment variables is @file{PATH}, it is a list of directories to search for executable names. Its value is a list of directories (separated by a colon, or `@key{:}'). When the address of the executable is not explicitly given (like @file{./configure} above), the system will look for the executable in the directories specified by @file{PATH}. If you have a computer nearby, try running the following command to see which directories your system will look into when it is searching for executable (binary) files, one example is printed here (notice how @file{/usr/bin}, in the @file{ls} example above, is one of the directories in @command{PATH}): @example $ echo $PATH /usr/local/sbin:/usr/local/bin:/usr/bin @end example By default @file{PATH} usually contains system-wide directories, which are readable (but not writable) by all users, like the above example. Therefore if you don't have root (or administrator) access, you need to add another directory to @file{PATH} which you actually have write access to. The standard directory where you can keep installed files (not just executables) for your own user is the @file{~/.local/} directory. The names of hidden files start with a `@key{.}' (dot), so it will not show up in your common command-line listings, or on the graphical user interface. You can use any other directory, but this is the most recognized. The top installation directory will be used to keep all the package's components: programs (executables), libraries, include (header) files, shared data (like manuals), or configuration files. So it commonly has some of the following sub-directories for each class of components respectively: @file{bin/}, @file{lib/}, @file{include/} @file{man/}, @file{share/}, @file{etc/}. Since the @file{PATH} variable is only used for executables, you can add the @file{~/.local/bin} directory to @file{PATH} with the following command. As defined below, first the existing value of @file{PATH} is used, then your given directory is added to its end and the combined value is put back in @file{PATH} (run `@command{$ echo $PATH}' afterwards to check if it was added). @example $ PATH=$PATH:~/.local/bin @end example @cindex GNU Bash @cindex Startup scripts @cindex Scripts, startup Any executable that you installed in this directory will now be usable without having to remember and type its full address. However, as soon as you leave your current terminal session, this modification will be lost. Adding your specified directory to the @file{PATH} environment variable each time you start a terminal is also very inconvenient and prone to errors. So there are standard `startup files' defined by your shell. There is a special startup file for every significant starting step: @table @asis @cindex GNU Bash @item @file{/etc/profile} and everything in @file{/etc/profile.d/} These startup scripts are called when your whole system starts (for example after you turn on your computer). Therefore you need administrator or root privileges to access or modify them. @item @file{~/.bash_profile} If you are using (GNU) Bash as your shell, the commands in this file are run once every time you log in to your account. @item @file{~/.bashrc} If you are using (GNU) Bash as your shell, the commands here will be run each time you start a terminal (for example, when you open your terminal emulator in the graphic user interface). @end table For security reasons, it is highly recommended to directly type in your @file{HOME} directory value by hand in startup files instead of using variables. So in the following, let's assume your user name is `@file{name}'. To add @file{~/.local/bin} to your @file{PATH} automatically on every startup you have to ``export'' the new value of @command{PATH} in the startup file that is most relevant to you with the line `@command{export PATH=$PATH:/home/name/.local/bin}'. You can either do it manually using a text editor, or by running the following command which will add this line as the last line of the file. Let's assume you want to add it to @file{~/.bashrc} (afterwards, open your @file{~/.bashrc} with a text editor and check it out to see for your self): @example $ echo 'export PATH=$PATH:/home/name/.local/bin' >> ~/.bashrc @end example @cindex GNU build system @cindex Install directory @cindex Directory, install Now that you know your system will look into @file{~/.local/bin} for executables, you can tell Gnuastro's configure script to install everything in the top @file{~/.local} directory using the @option{--prefix} option. The configure script will then put the executables in @file{~/.local/bin}, the compiled library files in @file{~/.local/lib}, the library header files in @file{~/.local/include} and so on (see @ref{Review of library fundamentals} for a review of the compiled library files and the headers). When you subsequently run @command{$ make install}, all the install-able files will be put in their respective directory under @file{~/.local/} (as discussed above). Note that tilde (`@key{~}') expansion will not happen if you put a `@key{=}' between @option{--prefix} and @file{~/.local}@footnote{If you insist on using `@key{=}', you can use @option{--prefix=$HOME/.local}.}, so we have avoided it here, see @ref{Options}. @example $ ./configure --prefix ~/.local @end example @cindex @file{MANPATH} @cindex @file{INFOPATH} @cindex @file{LD_LIBRARY_PATH} @cindex Library search directory @cindex Default library search directory You can install everything (including libraries like GSL, CFITSIO, or WCSLIB) locally by configuring them as above. However, recall that @command{PATH} is only for executable files, not libraries. Therefore, when building programs or libraries@footnote{For example WCSLIB which needs CFITSIO, or Gnuastro which needs both.} that depend on libraries you installed like this, you have to guide your compiler to the necessary directories. To do that, you have to define the @command{LDFLAGS} and @command{CPPFLAGS} environment variables respectively. This can be done while calling @file{./configure}: @example $ ./configure LDFLAGS=-L/home/name/.local/lib \ CPPFLAGS=-I/home/name/.local/include \ --prefix ~/.local @end example It can be annoying to do this when configuring every package, so you can define these two variables in a startup file (discussed above). The convention on using these variables doesn't include a colon to separate values (as @command{PATH}-like variables do), they use white space characters and each value is prefixed with a compiler option@footnote{These variables are ultimately used as options while building the programs, so every value has be an option name followed be a value as discussed in @ref{Options}.} (note the @option{-L} and @option{-I} above, see @ref{Options}). Therefore we have to keep the value in double quotation signs to keep the white space characters. Run the following two commands to do that if you want them in your @file{~/.bashrc}. @example echo 'export LDFLAGS="$LDFLAGS -L/home/name/.local/lib"' >> ~/.bashrc echo 'export CPPFLAGS="$CPPFLAGS -I/home/name/.local/include"' \ >> ~/.bashrc @end example To be able to link to the locally installed dynamic libraries (which are linked at run time) after installation, add @file{~/.local/lib} to your @command{LD_LIBRARY_PATH} environment variable similar to the example above for @command{PATH}. If you also want to access the Info (see @ref{Info}) and man pages (see @ref{Man pages}) documentations add @file{~/.local/share/info} and @file{~/.local/share/man} to your @command{INFOPATH}@footnote{Info has the following convention: ``If the value of @command{INFOPATH} ends with a colon [or it isn't defined] ..., the initial list of directories is constructed by appending the build-time default to the value of @command{INFOPATH}.'' So when installing in a non-standard directory and if @command{INFOPATH} was not initially defined, add a colon to the end of @command{INFOPATH} as shown below, otherwise Info will not be able to find system-wide installed documentation:@*@command{echo 'export INFOPATH=$INFOPATH:/home/name/.local/share/info:' >> ~/.bashrc}@* Note that this is only an internal convention of Info, do not use it for other @command{*PATH} variables.} and @command{MANPATH} environment variables. @cindex Search directory order @cindex Order in search directory A final note is that order matters in the directories that are searched for all the variables discussed above. In the examples above, the new directory was added after the system specified directories. So if the program, library or manuals are found in the system wide directories, the user directory is no longer searched. If you want to search your local installation first, put the new directory before the already existing list like the example below. @example export LD_LIBRARY_PATH=/home/name/.local/lib:$LD_LIBRARY_PATH @end example @noindent This is good when a library, for example CFITSIO, is already present on the system, but the system-wide install wasn't configured with the correct configuration flags (see @ref{CFITSIO}), or you want to use a newer version and you don't have administrator or root access to update it. With e above order @file{LD_LIBRARY_PATH}, the system will first find the CFITSIO you installed for yourself and will never reach the system-wide installation. However there are important security problems: because all important system-wide programs and libraries can be replaced by non-secure versions if they also exist in @file{./.local/}. So if you choose this order, be sure to keep it clean from executables or libraries with the same names as important system programs or libraries. @node Executable names, Configure and build in RAM, Installation directory, Configuring @subsubsection Executable names @cindex Executable names @cindex Names of executables At first sight, the names of the executables for each program might seem to be uncommonly long, for example @command{astnoisechisel} or @command{astimgcrop}. We could have chosen terse (and cryptic) names like most programs do. We chose this complete naming convention (something like the commands in @TeX{}) so you don't have to spend too much time remembering what the name of a specific program was. Such complete names also enable you to easily search for the programs. @cindex Shell auto-complete @cindex Auto-complete in the shell To facilitate typing the names in, we suggest using the shell auto-complete. With this facility you can find the executable you want very easily. It is very similar to file name completion in the shell. For example, simply by typing the letters below (where @key{[TAB]} stands for the Tab key on your keyboard) @example $ ast[TAB][TAB] @end example @noindent you will get the list of all the available executables that start with @command{ast} in your @command{PATH} environment variable directories. So, all the Gnuastro executables installed on your system will be listed. Typing the next letter for the specific program you want along with a Tab, will limit this list until you get to your desired program. @cindex Names, customize @cindex Customize executable names In case all of this does not convince you and you still want to type short names, some suggestions are given below. You should have in mind though, that if you are writing a shell script that you might want to pass on to others, it is best to use the standard name because other users might not have adopted the same customizations. The long names also serve as a form of documentation in such scripts. A similar reasoning can be given for option names in scripts: it is good practice to always use the long formats of the options in shell scripts, see @ref{Options}. @cindex Symbolic link The simplest solution is making a symbolic link to the actual executable. For example let's assume you want to type @file{ic} to run ImageCrop instead of @file{astimgcrop}. Assuming you installed Gnuastro executables in @file{/usr/local/bin} (default) you can do this simply by running the following command as root: @example # ln -s /usr/local/bin/astimgcrop /usr/local/bin/ic @end example @noindent In case you update Gnuastro and a new version of ImageCrop is installed, the default executable name is the same, so your custom symbolic link still works. @vindex --program-prefix @vindex --program-suffix @vindex --program-transform-name The installed executable names can also be set using options to @command{$ ./configure}, see @ref{Configuring}. GNU Autoconf (which configures Gnuastro for your particular system), allows the builder to change the name of programs with the three options @option{--program-prefix}, @option{--program-suffix} and @option{--program-transform-name}. The first two are for adding a fixed prefix or suffix to all the programs that will be installed. This will actually make all the names longer! You can use it to add versions of program names to the programs in order to simultaneously have two executable versions of a program. @cindex SED, stream editor @cindex Stream editor, SED The third configure option allows you to set the executable name at install time using the SED program. SED is a very useful `stream editor'. There are various resources on the internet to use it effectively. However, we should caution that using configure options will change the actual executable name of the installed program and on every re-install (an update for example), you have to also add this option to keep the old executable name updated. Also note that the documentation or configuration files do not change from their standard names either. @cindex Removing @file{ast} from executables For example, let's assume that typing @file{ast} on every invocation of every program is really annoying you! You can remove this prefix from all the executables at configure time by adding this option: @example $ ./configure --program-transform-name='s/ast/ /' @end example @node Configure and build in RAM, , Executable names, Configuring @subsubsection Configure and build in RAM @cindex File I/O @cindex Input/Output, file The configure and build process involves the creation, reading, and modification of a large number of files (input/output, or I/O). Therefore file I/O issues can directly affect the work of developers who need to configure and build Gnuastro numerous times. Some of these issues are listed below: @itemize @cindex HDD @cindex SSD @item I/O will cause wear and tear on both the HDDs (mechanical failures) and SSDs (decreasing the lifetime). @cindex Backup @item Having the built files mixed with the source files can greatly affect backing up (synchronization) of source files (since it involves the management of a large number of small files that are regularly changed. Backup software can of course be configured to ignore the built files and directories. However, since the built files are mixed with the source files and can have a large variety, this will require a high level of customization. @end itemize @cindex tmpfs file system @cindex file systems, tmpfs One solution to address both these problems is to use the @url{https://en.wikipedia.org/wiki/Tmpfs, tmpfs file system}. Any file in tmpfs is actually stored in the RAM (and possibly SAWP), not on HDDs or SSDs. The RAM is built for extensive and fast I/O. Therefore the large number of file I/Os associated with configuring and building will not harm the HDDs or SSDs. Due to the volatile nature of RAM, files in the tmpfs file-system will be permanently lost after a power-off. Since all configured and built files are derivative files (not files that have been directly written by hand) there is no problem in this and this feature can be considered as an automatic cleanup. @cindex Linux kernel @cindex GNU C library @cindex GNU build system The modern GNU C library (and thus the Linux kernel) define the @file{/dev/shm} directory for this purpose (POSIX shared memory). So using GNU Build System's ability to build in a separate directory (not necessarily in the source directory), we can configure and build the programs in @file{/dev/shm} to benefit from the RAM. To simplify the process, Gnuastro comes with a @file{tmpfs-config-make} script. This script will create a directory in the shared memory, and put a symbolic link to it (called @file{build}) in the top source directory (the backup/sync software therefore only needs to ignore this single link/file). The script will then internally change to that directory and configure and build (@command{make -kjN}, where @command{N} is the number of threads for a parallel build) Gnuastro in there. To benefit from this script, simply run the following command instead of @command{./configure} and @command{make}: @example $ ./tmpfs-config-make @end example @cindex GNU Emacs After this script is finished, you can `@command{cd build}' and run other Make commands (for example, `@command{make check}', `@command{make install}', or `@command{make pdf}') from there. In Emacs, the command to be run with the @command{M-x compile} command (by default: @command{make -k}) can be changed to `@command{cd build; make -kjN}', or `@command{make -C build -kjN}' (@command{N} is the number of threads; an integer @mymath{\geq1}). For subsequent builds (during development) the @command{M-x recompile} command will also do all the building in the RAM while you modify the clean, and backed-up source files and make minimal/efficient use of your non-volatile HDD or SSD. This script can be used in any software which is configured and built using the GNU Build System. Just copy it in the top source directory of that software and run it from there. The default number of threads and location of the shared memory (@file{/dev/shm}) are currently hard-coded within the script. If you need to change them, please open the script with a text editor and set their values manually. @node Tests, A4 print book, Configuring, Build and install @subsection Tests @cindex @command{make check} @cindex @file{mock.fits} @cindex Tests, running @cindex Checking tests After successfully building (compiling) the programs with the @command{$ make} command you can check the installation before installing. To run the tests, run @example $ make check @end example For every program some tests are designed to check some possible operations. Running the command above will run those tests and give you a final report. If everything is ok and you have built all the programs, all the tests should pass. In case any of the tests fail, please have a look at @ref{Known issues} and if that still doesn't fix your problem, look that the @file{./tests/test-suite.log} file to see if the source of the error is something particular to your system or more general. If you feel it is general, please contact us because it might be a bug. Note that the tests of some programs depend on the outputs of other program's tests, so if you have not installed them they might be skipped or fail. Prior to releasing every distribution all these tests are checked. If you have a reasonably modern terminal, the outputs of the successful tests will be colored green and the failed ones will be colored red. These scripts can also act as a good set of examples for you to see how the programs are run. All the tests are in the @file{tests/} directory. The tests for each program are shell scripts (ending with @file{.sh}) in a sub-directory of this directory with the same name as the program. See @ref{Test scripts} for more detailed information about these scripts in case you want to inspect them. @node A4 print book, Known issues, Tests, Build and install @subsection A4 print book @cindex A4 print book @cindex Modifying print book @cindex A4 paper size @cindex US letter paper size @cindex Paper size, A4 @cindex Paper size, US letter The default print version of this book is provided in the letter paper size. If you would like to have the print version of this book on paper and you are living in a country which uses A4, then you can rebuild the book. The great thing about the GNU build system is that the book source code which is in Texinfo is also distributed with the program source code, enabling you to do such customizations (hacking). @cindex GNU Texinfo In order to change the paper size, you will need to have GNU Texinfo installed. Open @file{doc/gnuastro.texi} with any text editor. This is the source file that created this book. In the first few lines you will see this line: @example @@c@@afourpaper @end example @noindent In Texinfo, a line is commented with @code{@@c}. Therefore, un-comment this line by deleting the first two characters such that it changes to: @example @@afourpaper @end example @noindent Save the file and close it. You can now run @example $ make pdf @end example @noindent and the new PDF book will be available in @file{SRCdir/doc/gnuastro.pdf}. By changing the @command{pdf} in @command{$ make pdf} to @command{ps} or @command{dvi} you can have the book in those formats. Note that you can do this for any book that is in Texinfo format, they might not have @code{@@afourpaper} line, so you can add it close to the top of the Texinfo source file. @node Known issues, , A4 print book, Build and install @subsection Known issues Depending on your operating system and the version of the compiler you are using, you might confront some known problems during the configuration (@command{$ ./configure}), compilation (@command{$ make}) and tests (@command{$ make check}). Here, their solutions are discussed. @itemize @cindex Configuration, not finding library @cindex Development packages @item @command{$ ./configure}: @emph{Configure complains about not finding a library even though you have installed it.} The possible solution is based on how you installed the package: @itemize @item From your distribution's package manager. Most probably this is because your distribution has separated the header files of a library from the library parts. Please also install the `development' packages for those libraries too. Just add a @file{-dev} or @file{-devel} to the end of the package name and re-run the package manager. This will not happen if you install the libraries from source. When installed from source, the headers are also installed. @item @cindex @command{LDFLAGS} From source. Then your linker is not looking where you installed the library. If you followed the instructions in this chapter, all the libraries will be installed in @file{/usr/local/lib}. So you have to tell your linker to look in this directory. To do so, add @command{LDFLAGS=-L/usr/local/lib} to the Gnuastro configure script. If you want to use the libraries for your other programming projects, then export this environment variable similar to the case for @file{LD_LIBRARY_PATH} explained below. @end itemize @item @vindex --enable-gnulibcheck @cindex Gnulib: GNU Portability Library @cindex GNU Portability Library (Gnulib) @command{$ make}: @emph{Complains about an unknown function on a non-GNU based operating system.} In this case, please run @command{$ ./configure} with the @option{--enable-gnulibcheck} option to see if the problem is from the GNU Portability Library (Gnulib) not supporting your system or if there is a problem in Gnuastro, see @ref{Gnuastro configure options}. If the problem is not in Gnulib and after all its tests you get the same complaint from @command{make}, then please contact us at @file{bug-gnuastro@@gnu.org}. The cause is probably that a function that we have used is not supported by your operating system and we didn't included it along with the source tar ball. If the function is available in Gnulib, it can be fixed immediately. @item @cindex @command{CPPFLAGS} @command{$ make}: @emph{Can't find the headers (.h files) of libraries installed from source.} Similar to the case for @file{LDFLAGS} (above), your compiler is not looking in the right place, add @command{CPPFLAGS=-I/usr/local/include} to @command{./configure} to re-configure Gnuastro, then re-run make. @item @cindex @code{rpl_malloc} @cindex GNU portability library @command{$ make check}: @emph{Complaint about @code{rpl_malloc} before the tests begin.} This is a problem with the different ways different operating systems implement C's @code{malloc} function. It doesn't happen when building Gnuastro with @command{$ make} because the GNU Portability Library (Gnulib) is used to compensate for the differences. But in @command{make check}, Gnulib is not used, so this error might pop-up there. To fix it, please re-run configure like below (adding any other options/arguments you might have already used): @example ./configure ac_cv_func_malloc_0_nonnull=yes @end example @cindex Tests, only one passes @cindex @file{LD_LIBRARY_PATH} @item @command{$ make check}: @emph{Only one @file{.sh} test passes, all the rest fail.} It is highly likely that your distribution doesn't look into the @file{/usr/local/lib} directory when searching for shared libraries. To make sure it is added to the list of directories, run the following command and restart your terminal: (you can ignore the @command{\} and extra space if you type it, it is only necessary if you copy and paste). See @ref{Installation directory} for more details. @example echo 'export LD_LIBRARY_PATH=$LD_LIBRARY_PATH:/usr/local/lib' \ >> ~/.bashrc @end example @cindex GPL Ghostscript @item @command{$ make check}: @emph{The tests relying on external programs (for example @file{fitstopdf.sh} fail.}) This is probably due to the fact that the version number of the external programs is too old for the tests we have preformed. Please update the program to a more recent version. For example to create a PDF image, you will need GPL Ghostscript, but older versions do not work, we have successfully tested it on version 9.15. Older versions might cause a failure in the test result. @item @cindex @TeX{} @cindex GNU Texinfo @command{$ make pdf}: @emph{The PDF book cannot be made.} To make a PDF book, you need to have the GNU Texinfo program (like any program, the more recent the better). A working @TeX{} program is also necessary, which you can get from Tex Live@footnote{@url{https://www.tug.org/texlive/}}. @item @cindex GNU Libtool After @code{make check}: do not copy the programs' executables to another (for example, the installation) directory manually (using @command{cp}, or @command{mv} for example). In the default configuration@footnote{If you configure Gnuastro with the @option{--disable-shared} option, then the libraries will be statically linked to the programs and this problem won't exist, see @ref{Linking}.}, the program binaries need to link with Gnuastro's shared library which is also built and installed with the programs. Therefore, to run successfully before and after installation, linking modifications need to be made by GNU Libtool at installation time. @command{make install} does this internally, but a simple copy might give linking errors when you run it. If you need to copy the executables, you can do so after installation. @end itemize @noindent If your problem was not listed above, please file a bug report (@ref{Report a bug}). @node Common program behavior, Extensions and Tables, Installation, Top @chapter Common program behavior There are some facts that are common to all the programs in Gnuastro which are mainly to do with user interaction. In this chapter these aspects are discussed. The most basic are the command-line options which are common in all the programs for a unified user experience. All Gnuastro programs can use configuration files so you don't have to specify all the parameters on the command-line each time you run a program. The manner of setting, checking and using the these files at various levels are also explained. Finally we discuss how you can get immediate and distraction-free (without taking your hands off the keyboard!) help on the command-line. @menu * Command-line:: How to use the command-line. * Configuration files:: Values for unspecified variables. * Threads in Gnuastro:: How threads are managed in Gnuastro. * Final parameter values:: The final set of used parameters. * Automatic output:: About automatic output names. * Getting help:: Getting more information on the go. * Output headers:: Common headers to all FITS outputs. @end menu @node Command-line, Configuration files, Common program behavior, Common program behavior @section Command-line All the programs in Gnuastro are customized through the standard GNU style command-line options. First a general outline of how to make best use of these options is discussed and finally the options that are common to all the programs in Gnuastro are listed. @cindex Metacharacters @cindex Token separation @cindex Command-line token separation @cindex Separating tokens on the command-line Your full command-line text is passed onto the shell as a string of characters. That string is then broken up into separate `words' by any `metacharacters' (like space, tab, @command{|}, @command{>} or @command{;}) that might exist in the text. See the GNU Bash manual, for the complete list of meta-characters and other Bash definitions. Its ``Shell Operation'' section has a short summary of the steps the shell takes before passing the commands to the program you called. @menu * Arguments and options:: Basics of options and arguments. * Arguments:: Treatment of arguments. * Options:: How to use GNU style options. * Common options:: Common options to all Gnuastro programs. @end menu @node Arguments and options, Arguments, Command-line, Command-line @subsection Arguments and options @cindex Options to programs @cindex Command-line options @cindex Arguments to programs @cindex Command-line arguments On the command-line, the first thing you enter is the name of the program you want to run. After that you can specify two types of input: @emph{arguments} and @emph{options}. Arguments are those tokens that are not preceded by any hyphens (@command{-}), the program is suppose to understand what they are without any help from the user. @vindex --help @vindex --usage @cindex Mandatory arguments Arguments can be both mandatory and optional and since there is no help from you, their order might also matter (for example in @command{cp} which is used for copying). The outputs of @option{--usage} and @option{--help} shows which arguments are optional and which are mandatory, see @ref{--usage}. As their name suggests, @emph{options} are only optional and most of the time you don't have to worry about what order you specify them in. @cindex Metacharacters on the command-line In case your arguments or option values contain any of the shell's meta-characters, you have to quote them. If there is only one such character, you can use a backslash (@command{\}) before it. If there are multiple, it might be easier to simply put your whole argument or option value inside of double quotes (@command{"}). In such cases, everything inside the double quotes will be seen as one `word'. @cindex HDU @cindex Header data unit For example let's say you want to specify the Header data unit (HDU) of your FITS file using a complex expression like @command{3; images(exposure > 100)}. If you simply add these after the @option{--hdu} (@option{-h}) option, the programs in Gnuastro will read the value to the HDU option as @command{3} and run. Then, Bash will attempt to run a separate command @command{images(exposure > 100)} and complain about a syntax error. This is because the semicolon (@command{;}) is an `end of command' character in Bash. To solve this problem you can simply put double quotes around the whole string you want to pass as seen below: @example $ astimgcrop --hdu="3; images(exposure > 100)" FITSimage.fits @end example Alternatively you can put a @command{\} before every metacharacter in this string, but probably you will agree with us that the double quotes are much more easier, elegant and readable. @node Arguments, Options, Arguments and options, Command-line @subsection Arguments In Gnuastro, the names of the input data files and ASCII tables are mostly specified as arguments, you can generally specify them in any order unless otherwise stated for a particular program. Everything particular about how a program treats arguments, is explained under the ``Invoking ProgramName'' section for that program. Generally, if there is a standard file name extension for a particular format, that filename extension is used to separate the kinds of arguments. The list below shows what astronomical data formats are recognized based on their file name endings. If the program doesn't accept any other data format, any other argument that doesn't end with the specified extensions below is considered to be a text file (usually catalogs). For example @ref{ConvertType} accepts other data formats. @cindex Astronomical data suffixes @cindex Suffixes, astronomical data @itemize @item @file{.fits}: The standard file name ending of a FITS image. @item @file{.fits.Z}: A FITS image compressed with @command{compress}. @item @file{.fits.gz}: A FITS image compressed with GNU zip (gzip). @item @file{.fits.fz}: A FITS image compressed with @command{fpack}. @item @file{.imh}: IRAF format image file. @end itemize Through out this book and in the command-line outputs, whenever we want to generalize all such astronomical data formats in a text place holder, we will use @file{ASTRdata}, we will assume that the extension is also part of this name. Any file ending with these names is directly passed on to CFITSIO to read. Therefore you don't necessarily have to have these files on your computer, they can also be located on an FTP or HTTP server too, see the CFITSIO manual for more information. CFITSIO has its own error reporting techniques, if your input file(s) cannot be opened, or read, those errors will be printed prior to the final error by Gnuastro. @node Options, Common options, Arguments, Command-line @subsection Options @cindex GNU style options @cindex Options, GNU style @cindex Options, short (@option{-}) and long (@option{--}) Command-line options allow configuring the behavior of a program in all GNU/Linux applications for each particular execution. Most options can be called in two ways: @emph{short} or @emph{long} a small number of options in some programs only have the latter type. In the list of options provided in @ref{Common options} or those for each program, both formats are shown for those which support both. First the short is shown then the long. Short options are only one character and only have one hyphen (for example @option{-h}) while long options have two hyphens an can have many characters (for example @option{--hdu}). Usually, the short options are for when you are writing on the command line and want to save keystrokes and time. The long options are good for shell scripts, where you don't usually have a rush and they provide a level of documentation, since they are less cryptic. Usually after a few months of not running a program, the short options will be forgotten and reading your previously written script will not be easy. @cindex On/Off options @cindex Options, on/off Some options need to be given a value if they are called and some don't. You can think of the latter type of options as on/off options. These two types of options can be distinguished using the output of the @option{--help} and @option{--usage} options, which are common to all GNU software, see @ref{Getting help}. The following convention is used for the formats of the values in Gnuastro: @vtable @option @item INT The value is read as an integer. If a float or a string is provided the program will warn you and abort. In most cases, integers are used for counting variables, so if they are negative the program will also abort. @item 4or8 Either the value 4 or 8, any other integer will give a warning and abort. @item FLT The value is read as a float. There are generally two types, depending on the context. If they are for fractions, they will have to be less than or equal to unity. @item STR The value is read as a string of characters (for example a file name) or other particular settings like a HDU name, see below. @end vtable @noindent @cindex Values to options @cindex Option values To specify a value in the short format, simply put the value after the option. Note that since the short options are only one character long, you don't have to type anything between the option and its value. For the long option you either need white space or an @option{=} sign, for example @option{-h2}, @option{-h 2}, @option{--hdu 2} or @option{--hdu=2} are all equivalent. The short format of on/off options (those that don't need values) can be concatenated for example these two hypothetical sequences of options are equivalent: @option{-a -b -c4} and @option{-abc4}. As an example, consider the following command to run ImageCrop: @example $ astimgcrop -Dr3 --wwidth 3 catalog.txt --deccol=4 ASTRdata @end example @noindent The @command{$} is the shell prompt, @command{astimgcrop} is the program name. There are two arguments (@command{catalog.txt} and @command{ASTRdata}) and four options, two of them given in short format (@option{-D}, @option{-r}) and two in long format (@option{--width} and @option{--deccol}). Three of them require a value and one (@option{-D}) is an on/off option. @vindex --printparams @cindex Options, abbreviation @cindex Long option abbreviation If an abbreviation is unique between all the options of a program, the long option names can be abbreviated. For example, instead of typing @option{--printparams}, typing @option{--print} or maybe even @option{--pri} will be enough, if there are conflicts, the program will warn you and show you the alternatives. Finally, if you want the argument parser to stop parsing arguments beyond a certain point, you can use two dashes: @option{--}. No text on the command-line beyond these two dashes will be parsed. @cindex Repeated options @cindex Options, repeated If an option with a value is repeated or called more than once, the value of the last time it was called will be assigned to it. This very useful in complicated situations, for example in scripts. Let's say you want to make a small modification to one option value. You can simply type the option with a new value in the end of the command and see how the script works. If you are satisfied with the change, you can remove the original option. If the change wasn't satisfactory, you can remove the one you just added and not worry about saving the original value. Without this capability, you would have to memorize or save the original value somewhere else, run the command and then change the value again which is not at all convenient and is potentially cause lots of bugs. @cindex Configuration files @cindex Default option values When you don't call an option that requires a value, all the programs in Gnuastro will check configuration files to find a value for that parameter. To learn more about how folder, user and system wide configuration files can be set, please see @ref{Configuration files}. Another factor that is particular to Gnuastro is that it will check the value you have given for each option to see if it is reasonable. For example you might mistakenly give a negative, float or string value for a FITS image extension or column number. As another example, you might give a value larger than unity for an option that only accepts fractions (which are always less than unity and positive). @cartouche @noindent @cindex Tilde expansion as option values @strong{CAUTION:} In specifying a file address, if you want to use the shell's tilde expansion (@command{~}) to specify your home directory, leave at least one space between the option name and your value. For example use @command{-o ~/test}, @command{--output ~/test} or @command{--output= ~/test}. Calling them with @command{-o~/test} or @command{--output=~/test} will disable shell expansion. @end cartouche @cartouche @noindent @strong{CAUTION:} If you forget to specify a value for an option which requires one, and that option is the last one, Gnuastro will warn you. But if it is in the middle of the command, it will take the text of the next option or argument as the value which can cause undefined behavior. @end cartouche @cartouche @noindent @cindex Counting from zero. @strong{NOTE:} All counting in Gnuastro starts from 0 not 1. So for example the first FITS image extension or column in a table are noted by 0, not 1. This is the standard in C and all languages that are based on it (for example C++, Java and Python). @end cartouche @node Common options, , Options, Command-line @subsection Common options @cindex Options common to all programs @cindex Gnuastro common options To facilitate the job of the users and developers, all the programs in Gnuastro share some basic command-line options for the same operations where they are relevant. The list of options is provided below. It is noteworthy that these similar options are hard-wired into the programming of all of Gnuastro programs using GNU C library's argument parser merging ability. @cindex Irrelevant options @cindex Options, irrelevant For some programs, some of the options, might be irrelevant for example MakeProfiles creates FITS images based on a given catalog. Therefore no input images (and thus HDUs) are necessary for it. In such cases, the option is still listed and if a value is given for it, it is completely ignored. @menu * Input output:: Common input/output options. * Operating modes:: Common operating mode options. @end menu @node Input output, Operating modes, Common options, Common options @subsubsection Input/Output options These options are to do with the input and outputs of the various programs. @vtable @option @cindex HDU @cindex Header data unit @item -h @itemx --hdu (@option{=STR}) The number or name of the desired Header Data Unit or HDU in the input FITS image or images. A FITS file can store multiple HDUs or extensions, each with either an image or a table or nothing at all (only a header). Note that counting of the extensions starts from 0(zero), not 1(one). When specifying the name, case is not important so @command{IMAGE}, @command{image} or @command{ImAgE} are equivalent. A @code{#} is appended to the string you specify for the HDU@footnote{With the @code{#} character, CFITSIO will only read the desired HDU into your memory, not all the existing HDUs in the fits file.} and the result is put in square brackets and appended to the FITS file name before calling CFITSIO to read the contents of the HDU for all the programs in Gnuastro. CFITSIO has many capabilities to help you find the extension you want, far beyond the simple extension number and name. See CFITSIO manual's ``HDU Location Specification'' section for a very complete explanation with several examples. Note that in some programs, the behavior of @option{--hdu} might be different, for example see @ref{Invoking astarithmetic}, were it can be called multiple times and the value of each all will be stored. @item -o @itemx --output (@option{=STR}) The name of the output file or directory. With this option the automatic output names explained in @ref{Automatic output} are ignored. @item -D @itemx --dontdelete By default, if the output file already exists, it will be silently replaced with the output of this run of all Gnuastro programs. By calling this option, if the output file already exists, the programs will warn you and abort. @item -K @itemx --keepinputdir In automatic output names, don't remove the directory information of the input file names. As explained in @ref{Automatic output}, if no output name is specified, then the output name will be made in the existing directory based on your input. If you call this option, the directory information of the input will be kept and the output will be in the same directory as the input. Note that his is only relevant if you are running the program from another directory! @end vtable @node Operating modes, , Input output, Common options @subsubsection Operating modes Another group of options that are common to all the programs in Gnuastro are those to do with the general operation of the programs. The explanation for those that are not only limited to Gnuastro but can be called in all GNU programs start with (GNU option). @vtable @option @item -- (GNU option) Stop parsing the command-line. This option can be useful in scripts or when using the shell history. Suppose you have a long list of options, and want to see if removing some of them (and using the default values) can give a better result. If the ones you want to remove are the last ones on the command-line, you don't have to delete them, you can just add @option{--} before them and if you don't get what you want, you can remove the @option{--} and get the same initial result. @item --usage (GNU option) Only print the options and arguments. This is very useful for when you know the what the options do, you have just forgot their names. See @ref{--usage}. @item -? @itemx --help (GNU option) Print all options and an explanation. Adding this option will print all the options in their short and long formats, also displaying which ones need a value if they are called (with an @option{=} after the long format). A short explanation is also given for what the option is for. The program will quit immediately after the message is printed and will not do any form of processing. See @ref{--help}. @item -V @itemx --version (GNU option) Print a short message, showing the full name, version, copyright information and program authors. On the first line it will print the official name (not executable name) and version number of the program. It will also print the version of the Gnuastro that the program was built with. Following this is a blank line and a copyright information. The program will not run. @item -q @itemx --quiet Don't report steps. All the programs in Gnuastro that have multiple major steps will report their steps for you to follow while they are operating. If you do not want to see these reports, you can call this option and only error messages will be printed if the program is aborted. If the steps are done very fast (depending on the properties of your input) disabling these reports will also decrease running time. @item --cite Print the Bib@TeX{} entry for Gnuastro and the particular program (if that program comes with a separate paper) and abort. Citations are vital for the continued work on Gnuastro. Gnuastro started and is continued based on separate research projects. So if you find any of the tools offered in Gnuastro to be useful in your research, please use the output of this command to cite the program and Gnuastro in your research paper. Thank you. Gnuastro is still new, there is no separate paper only devoted to Gnuastro yet. Therefore currently the paper to cite for Gnuastro is the paper for NoiseChisel which is the first published paper introducing Gnuastro to the astronomical community. Upon reaching a certain point, a paper completely devoted to Gnuastro will be published, see @ref{GNU Astronomy Utilities 1.0}. @item -P @itemx --printparams Print the final values used for all the parameters and abort. See @ref{Final parameter values} for more details. @item -S @itemx --setdirconf Update the current directory configuration file from the given command line options and quit, see @ref{Configuration files}. The values of your options are added to the configuration file in the current directory. If the configuration file or folder doesn't exist, it will be created. If it exists but has different values for those options, they will be given the new values. In any case, the program will not run, but the contents of its updated configuration file are printed for you to inspect. This is the recommended method to fill the configuration file for all future calls to one of the Gnuastro programs in a folder. It will internally check if your values are in the correct range and type and save them according to the configuration file format, see @ref{Configuration file format}. When this option is called, the otherwise mandatory arguments, for example input image or catalog file(s), are no longer mandatory (since the program will not run). @item -U @itemx --setusrconf Update the user configuration file from the command-line options and quit. See explanation under @option{--setdirconf} for more details. @item --onlydirconf Only read the current (local) directory configuration file and ignore the rest of the configuration files, see @ref{Configuration file precedence} and @ref{Current directory and User wide}. This can be very useful when you want your results to be exactly reproducible. All the configuration files can be put in the hidden @file{./.gnuastro/} directory in the current directory, or the hidden directory can be a symbolic link to the directory containing the configuration files. Then with this option you can ensure that no other configuration file is read. So if your local configuration file lacks some parameters, which ever Gnuastro program you are using will will warn you and abort, enabling you to exactly set all the necessary parameters without unknowingly relying on some user or system wide option values. @option{onlydirconf} can also be used in the configuration files (with a value of @option{0} or @option{1}), see @ref{Configuration file format}. If it is present in the local configuration file, other configuration files will not be read. In the other configuration files, it is irrelevant. @item --onlyversion (@option{=STR}) Only run the program if its version is equal with the string of characters given to this option. Note that it is not compared as a number, but as a string of characters, so @option{0}, or @option{0.0} and @option{0.00} are different. This is useful if you want your results to be exactly reproducible and not mistakenly run with an updated or older version of the program. @item --nolog For programs which generate Log files, if this option is called, no Log file will be generated. @cindex CPU threads, set number @cindex Number of CPU threads to use @item -N @itemx --numthreads (@option{=INT}) Set the number of CPU threads to use. See @ref{Threads in Gnuastro}. @end vtable @node Configuration files, Threads in Gnuastro, Command-line, Common program behavior @section Configuration files @cindex @file{etc} @cindex Configuration files @cindex Necessary parameters @cindex Default option values @cindex File system Hierarchy Standard Each program needs a certain number of parameters to run. Supplying all the necessary parameters each time you run the program is very frustrating and prone to errors. Therefore all the programs read the values for the necessary options you have not given in the command line from one of several plain text files (which you can view and edit with any text editor). These files are known as configuration files and are usually kept in a directory named @file{etc/} according to the file system hierarchy standard@footnote{@url{http://en.wikipedia.org/wiki/Filesystem_Hierarchy_Standard}}. @vindex --output @vindex --numthreads @cindex CPU threads, number @cindex Internal default value @cindex Number of CPU threads to use The thing to have in mind is that none of the programs in Gnuastro keep any internal default value. All the values must either be stored in one of the configuration files or explicitly called in the command-line. In case the necessary parameters are not given through any of these methods, the program will list the missing necessary parameters and abort. The only exception to this is @option{--numthreads}, whose default value is determined at run-time using the number of threads available to your system, see @ref{Threads in Gnuastro}. Of course, you can still provide a default value for the number of threads at any of the levels below, but if you don't, the program will not abort. Also note that through automatic output name generation, the value to the @option{--output} option is also not mandatory on the command-line or in the configuration files for all programs which don't rely on that value as an input@footnote{One example of a program which uses the value given to @option{--output} as an input is ConvertType, this value specifies the type of the output through the value to @option{--output}, see @ref{Invoking astconvertt}.}, see @ref{Automatic output}. @menu * Configuration file format:: ASCII format of configuration file. * Configuration file precedence:: Precedence of configuration files. * Current directory and User wide:: Local and user configuration files. * System wide:: System wide configuration files. @end menu @node Configuration file format, Configuration file precedence, Configuration files, Configuration files @subsection Configuration file format @cindex Configuration file suffix The configuration files for each program have the standard program executable name with a @file{.conf} suffix. When you download the source code, you can find them in the same directory as the source code of each program, see @ref{Program source}. @cindex White space character @cindex Configuration file format Any line in the configuration file whose first non-white character is a @key{#} is considered to be a comment and is ignored. The same goes for an empty line. The name of the parameter is the same as the long format of the command-line option for that parameter. The parameter name and parameter value have to be separated by any number of `white-space' characters: space, tab or vertical tab. By default several space characters are used. If the value of an option has space characters (most commonly for the @option{hdu} option), then double quotes can be used to specify the full value. In each non-commented and non-blank line, any text after the first two words (given the conditions above) is ignored. If it is an option without a value in the @option{--help} output (on/off option, see @ref{Options}), then the value should be @option{1} if it is to be `on' and @option{0} otherwise. If an option is not recognized in the configuration file, the name of the file and unrecognized option will be reported and the program will abort. If a parameter is repeated more more than once in the configuration files and it is not set on the command-line, then only the first value will be used, the rest will be ignored. @cindex Writing configuration files @cindex Automatic configuration file writing @cindex Configuration files, writing You can build or edit any of the directories and the configuration files yourself using any text editor. However, it is recommended to use the @option{--setdirconf} and @option{--setusrconf} options to set default values for the current directory or this user, see @ref{Operating modes}. With these options, the values you give will be checked as explained in @ref{Options} before writing in the current directory's configuration file. They will also print a set of commented lines guiding the reader and will also classify the options based on their context and write them in their logical order to be more understandable. @node Configuration file precedence, Current directory and User wide, Configuration file format, Configuration files @subsection Configuration file precedence @cindex Configuration file precedence @cindex Configuration file directories @cindex Precedence, configuration files The parameter values in all the programs of Gnuastro will be filled in the following order. Such that if a parameter is assigned a value in an earlier step, any value for that parameter in a later step will be ignored. @enumerate @item Command-line options, for this particular execution. @item Current directory, for all executions in the directory from which any of the programs is run (@file{./.gnuastro/}). @item The user's home directory, for all the executions of a particular user: (@file{$HOME/.local/etc/}, see below). It is only read if @option{--onlydirconf} is not called, see @ref{Operating modes}. @item In a system wide directory for any user on that computer (@file{prefix/etc/}, see @ref{Installation directory} for the value of @file{prefix}). It is only read if @option{--onlydirconf} is not called, see @ref{Operating modes}. @end enumerate @noindent The basic idea behind setting this progressive state of checking for parameter values is that separate users of a computer or separate folders in a user's file system might need different values for some parameters and the same values for others. For example raw telescope images usually have their main image extension in the second FITS extension, while processed FITS images usually only have one extension. If your system wide default input extension is 0 (the first), then when you want to work with the former group of data you have to explicitly mention it to the programs every time. With this progressive state of default values to check, you can set different default values for the different directories that you would like to run Gnuastro in for your different purposes, so you won't have to worry about this issue any more. @node Current directory and User wide, System wide, Configuration file precedence, Configuration files @subsection Current directory and User wide @cindex @file{HOME} @cindex @file{./.gnuastro/} @cindex @file{HOME/.local/etc/} For the current (local) and user-wide directories, the configuration files are stored in the hidden sub-directories named @file{./.gnuastro/} and @file{HOME/.local/etc/} respectively. Unless you have changed it, the @file{HOME} environment variable should point to your home directory. You can check it by running @command{$ echo $HOME}. Each time you run any of the programs in Gnuastro, this environment variable is read and placed in the above address. So if you suddenly see that your home configuration files are not being read, probably you (or some other program) has changed the value of this environment variable. @vindex --setdirconf @vindex --setusrconf Although it might cause confusions like above, this dependence on the @file{HOME} environment variable enables you to temporarily use a different directory as your home directory. This can come in handy in complicated situations. To set the user or current directory configuration files based on your command-line input, you can use the @option{--setdirconf} or @option{--setusrconf}, see @ref{Operating modes} @node System wide, , Current directory and User wide, Configuration files @subsection System wide @cindex @file{prefix/etc/} @cindex System wide configuration files @cindex Configuration files, system wide When Gnuastro is installed, the configuration files that are shipped with the distribution are copied into the (possibly system wide) @file{prefix/etc/} directory. See @ref{Configuring} for more details on @file{prefix} (by default it is: @file{/usr/local}). This directory is the final place (with the lowest priority) that the programs in Gnuastro will check to retrieve parameter values. If you remove a parameter and its value from the files in this system wide directory, you either have to specify it in more immediate configuration files or set it each time in the command-line. Recall that none of the programs in Gnuastro keep any internal default values and will abort if they don't find a value for the necessary parameters (except the number of threads). So even though you might never use a parameter, it still has to be at least available in this system-wide configuration file. In case you install Gnuastro from your distribution's repositories, @file{prefix} will either be set to @file{/} (the root directory) or @file{/usr}, so you can find the system wide configuration variables in @file{/etc/} or @file{/usr/etc/}. The prefix of @file{/usr/local/} is conventionally used for programs you install from source by your self. @node Threads in Gnuastro, Final parameter values, Configuration files, Common program behavior @section Threads in Gnuastro @pindex nproc @cindex pthread @cindex CPU threads @cindex GNU Coreutils @cindex Using CPU threads @cindex POSIX threads library @cindex CPU, using all threads @cindex Multi-threaded programs @cindex Using multiple CPU cores Some of the programs benefit significantly when you use all the threads your computer's CPU has to offer to your operating system. GNU Astronomy Utilities uses the POSIX threads library (pthreads) for spinning off threads when the user asks for it. The number of threads available to your operating system is usually double the number of physical (hardware) cores in your CPU. On a GNU/Linux system, the number of threads available can be found with the command @command{$ nproc} command (part of GNU Coreutils). @vindex --numthreads @cindex Number of threads available @cindex Available number of threads @cindex Internally stored option value Gnuastro can find the number of threads available to your system at run-time (when you execute the program). However, if a value is given provided for the @option{--numthreads} option, the given value will be used, not the value automatically read from your system, see @ref{Operating modes} and @ref{Configuration files} for ways to set a different value. Thus @option{--numthreads} is the only option with a value that doesn't have to be specified anywhere on the command-line or in the options. @menu * A note on threads:: Caution and suggestion on using threads. * How to run simultaneous operations:: How to run things simultaneously. @end menu @node A note on threads, How to run simultaneous operations, Threads in Gnuastro, Threads in Gnuastro @subsection A note on threads @cindex Using multiple threads @cindex Best use of CPU threads @cindex Efficient use of CPU threads Spinning off threads internally is not necessarily always the most efficient way to run an application. Creating a new thread isn't a cheap operation for the operating system. It is most useful when the input data are fixed and you want the same operation to be done on parts of it. For example one input image to ImageCrop and multiple crops from various parts of it. In this fashion, the image is loaded into memory once, all the crops are divided between the number of threads internally and each thread cuts out those parts which are assigned to it from the same image. On the other hand, if you have multiple images and you want to crop the same region out of all of them, it is much more efficient to set @option{--numthreads=1} (so no threads spin off) and run ImageCrop multiple times simultaneously, see @ref{How to run simultaneous operations}. @cindex Wall-clock time You can check the boost in speed by first running a program on one of the data sets with the maximum number of threads and another time (with everything else the same) and only using one thread. You will notice that the wall-clock time (reported by most programs at their end) in the former is longer than the latter divided by number of physical CPU cores available to your operating system. Asymptotically these two can be equal (most of the time they aren't). So limiting the programs to use only one thread and running them independently on the number of available threads will be more efficient. @cindex System Cache @cindex Cache, system Note that the operating system keeps a cache of recently processed data, so usually, the second time you process an identical data set (independent of the number of threads used), you will get faster results. In order to make an unbiased comparison, you have to first clean the system's cache with the following command between the two runs. @example $ sync; echo 3 | sudo tee /proc/sys/vm/drop_caches @end example @cartouche @noindent @strong{SUMMARY: Should I use multiple threads?} Depends: @itemize @item If you only have @strong{one} data set (image in most cases!), then yes, the more threads you use (with a maximum of the number of threads available to your OS) the faster you will get your results. @item If you want to run the same operation on @strong{multiple} data sets, it is best to set the number of threads to 1 and use GNU Parallel as explained above. @end itemize @end cartouche @node How to run simultaneous operations, , A note on threads, Threads in Gnuastro @subsection How to run simultaneous operations There are two approaches to simultaneously execute a program: using GNU Parallel or Make (GNU Make is the most common implementation). The first is very useful when you only want to do one job multiple times and want to get back to your work without actually keeping the command you ran. The second is usually for (very) complicated processes, with lots of dependencies between the different products (for example a data-production pipeline). @table @asis @item GNU Parallel @cindex GNU Parallel When you only want to run multiple instances of a command on different threads and get on with the rest of your work, the best method is to use GNU parallel. Surprisingly GNU Parallel is one of the few GNU packages that has no Info documentation but only a Man page, see @ref{Info}. So to see the documentation after installing it please run @example $ man parallel @end example @noindent As an example, let's assume we want to crop a region fixed on the pixels (500, 600) with the default width from all the FITS images in the @file{./data} directory ending with @file{sci.fits} to the current directory. To do this, you can run: @example $ parallel astimgcrop --numthreads=1 --xc=500 --yc=600 ::: \ ./data/*sci.fits @end example @noindent GNU Parallel can help in many more conditions, this is one of the simplest, see the man page for lots of other examples. For absolute beginners: the backslash (@command{\}) is only a line breaker to fit nicely in the page. If you type the whole command in one line, you should remove it. @item Make Make is a program built for specifying ``targets'', ``prerequisites'' and ``recipes''. It allows you to define very complicated dependency structures for complicated processes that commonly start off with a large list of inputs and builds them based on the dependencies you define. GNU Make@footnote{@url{https://www.gnu.org/software/make/}} is the most common implementation which (like nearly all GNU programs comes with a wonderful manual@footnote{@url{https://www.gnu.org/software/make/manual/}}). It is very basic and short (the most important part is about 100 pages). Make has the @option{--jobs} (@option{-j}) which allows you to specify the maximum number of jobs that can be done simultaneously. For example a common 4 physical core CPU usually has 8 processing threads. So you can run: @example $ make -j8 @end example Once the dependency tree for your processes is built, Make will run the independent targets simultaneously. @end table @node Final parameter values, Automatic output, Threads in Gnuastro, Common program behavior @section Final parameter values, reproduce previous results @vindex -P @vindex --printparams @cindex Final parameter value checking @cindex Checking final parameter values The input parameters can be specified in many places, either on the command-line or in at least one of several configuration files, see @ref{Configuration files}. Therefore, it often happens that before running a program on a certain data set, you want to see the values for the parameters that the program will use after it has read your command-line options and all the configuration files in their correct order. You might also want to save the list with the output so you can reproduce the same results at a later time, this is very important when you want to use your results in a report or paper. If you call the @option{--printparams} option, all Gnuastro programs will read your command-line parameters and all the configuration files. If there is no problem (like a missing parameter or a value in the wrong format) and immediately before actually running, the programs will print the full list of parameter names and values sorted and grouped by context and quit. They will also report their version number, the date they were configured on your system and the time they were reported. As an example, you can give your full command-line options and even the input and output file names and finally just add @option{-P} to check if all the parameters are finely set. If everything is ok, you can just run the same command (easily retrieved from the bash history, with the top arrow key) and simply remove the last two characters that showed this option. Since no program will actually start its processing when this option is called, the otherwise mandatory arguments for each program (for example input image or catalog files) are no longer required when you call this option. @cindex Bash history @cindex Shell redirection @cindex Redirection of output In case you want to store the list of parameters for later reproduction of the same results, you can do so with the GNU Bash re-direction tool. For example after you have produced the results you want to store, you can save all the parameters that were used in a file named @file{parameters.txt} in the following manner. Using shell history you can retrieve the last command you entered and simply add @command{-P > parameters.txt} to it, for example: @example $ astimgcrop --racol=2 --deccol=3 IN.fits cat.txt -P > parameters.txt @end example @cindex Reproducible results @noindent All the parameters along with the extra data explained before will be stored in the plain text @file{parameters.txt} file through the shell's redirection mechanism (@command{>}). The output of @option{--printparams} conforms with the configuration file formats@footnote{They are both written by the same function.}. By taking the following steps, you can use this file as a configuration file to reproduce your results at a later time. @enumerate @item Set the file name based on the standard configuration file names, see @ref{Configuration file format}. @item Later on (when ever you want to re-produce your results), copy the file in the @file{./.gnuastro/} directory of your current directory. @end enumerate @noindent In this manner, this file will be read as a current directory configuration file and since all the parameters are defined in it, no other configuration file value will be used. @node Automatic output, Getting help, Final parameter values, Common program behavior @section Automatic output @cindex Automatic output file names @cindex Output file names, automatic @cindex Setting output file names automatically All the programs in Gnuastro are designed such that specifying an output file or directory (based on the program context) is optional. The outputs of most programs are automatically found based on the input and what the program does. For example when you are converting a FITS image named @file{FITSimage.fits} to a JPEG image, the JPEG image will be saved in @file{FITSimage.jpg}. @vindex --keepinputdir Another very important part of the automatic output generation is that all the directory information of the input file name is stripped off of it. This feature can be disabled with the @option{--keepinputdir} option, see @ref{Common options}. It is the default because astronomical data are usually very large and organized specially with special file names. In some cases, the user might not have write permissions in those directories. In fact, even if the data is stored on your own computer, it is advised to only grant write permissions to the super user or root. This way, you won't accidentally delete or modify your valuable data! Let's assume that we are working on a report and want to process the FITS images from two projects (ABC and DEF), which are stored in the sub-directories named @file{ABCproject/} and @file{DEFproject/} of our top data directory (@file{/mnt/data}). The following shell commands show how one image from the former is first converted to a JPEG image through ConvertType and then the objects from an image in the latter project are detected using NoiseChisel. The text after the @command{#} sign are comments (not typed!). @example $ pwd # Current location /home/usrname/research/report $ ls # List directory contents ABC01.jpg $ ls /mnt/data/ABCproject # Archive 1 ABC01.fits ABC02.fits ABC03.fits $ ls /mnt/data/DEFproject # Archive 2 DEF01.fits DEF02.fits DEF03.fits $ astconvertt /mnt/data/ABCproject/ABC02.fits --output=jpg # Prog 1 $ ls ABC01.jpg ABC02.jpg $ astnoisechisel /mnt/data/DEFproject/DEF01.fits # Prog 2 $ ls ABC01.jpg ABC02.jpg DEF01_labeled.fits @end example @node Getting help, Output headers, Automatic output, Common program behavior @section Getting help @cindex Help @cindex Book formats @cindex Remembering options @cindex Convenient book formats Probably the first time you read this book, it is either in the PDF or HTML formats. These two formats are very convenient for when you are not actually working, but when you are only reading. Later on, when you start to use the programs and you are deep in the middle of your work, some of the details will inevitably be forgotten. Going to find the PDF file (printed or digital) or the HTML webpage is a major distraction. @cindex Online help @cindex Command-line help GNU software have a very unique set of tools for aiding your memory on the command-line, where you are working, depending how much of it you need to remember. In the past, such command-line help was known as ``online'' help, because they were literally provided to you `on' the command `line'. However, nowadays the word ``online'' refers to something on the internet, so that term will not be used. With this type of help, you can resume your exciting research without taking your hands off the keyboard. @cindex Installed help methods Another major advantage of such command-line based help routines is that they are installed with the software in your computer, therefore they are always in sync with the executable you are actually running. Three of them are actually part of the executable. You don't have to worry about the version of the book or program. If you rely on external help (a PDF in your personal print or digital archive or HTML from the official webpage) you have to check to see if their versions fit with your installed program. If you only need to remember the short or long names of the options, @option{--usage} is advised. If it is what the options do, then @option{--help} is a great tool. Man pages are also provided for those who are use to this older system of documentation. This full book is also available to you on the command-line in Info format. If none of these seems to resolve the problems, there is a mailing list which enables you to get in touch with experienced Gnuastro users. In the subsections below each of these methods are reviewed. @menu * --usage:: View option names and value formats. * --help:: List all options with description. * Man pages:: Man pages generated from --help. * Info:: View complete book in terminal. * help-gnuastro mailing list:: Contacting experienced users. @end menu @node --usage, --help, Getting help, Getting help @subsection @option{--usage} @vindex --usage @cindex Usage pattern @cindex Mandatory arguments @cindex Optional and mandatory tokens If you give this option, the program will not run. It will only print a very concise message showing the options and arguments. Everything within square brackets (@option{[]}) is optional. For example here are the first and last two lines of ImageCrop's @option{--usage} is shown: @example $ astimgcrop --usage Usage: astimgcrop [-Do?IPqSVW] [-d INT] [-h INT] [-r INT] [-w INT] [-x INT] [-y INT] [-c INT] [-p STR] [-N INT] [--deccol=INT] .... [--setusrconf] [--usage] [--version] [--wcsmode] [ASCIIcatalog] FITSimage(s).fits @end example There are no explanations on the options, just their short and long names shown separately. After the program name, the short format of all the options that don't require a value (on/off options) is displayed. Those that do require a value then follow in separate brackets, each displaying the format of the input they want, see @ref{Options}. Since all options are optional, they are shown in square brackets, but arguments can also be optional. For example in this example, a catalog name is optional and is only required in some modes. This is a standard method of displaying optional arguments for all GNU software. @node --help, Man pages, --usage, Getting help @subsection @option{--help} @vindex --help If the command-line includes this option, the program will not be run. It will print a complete list of all available options along with a short explanation. The options are also grouped by their context. Within each context, the options are sorted alphabetically. Since the options are shown in detail afterwards, the first line of the @option{--help} output shows the arguments and if they are optional or not, similar to @ref{--usage}. In the @option{--help} output of all programs in Gnuastro, the options for each program are classified based on context. The first two contexts are always options to do with the input and output respectively. For example input image extensions or supplementary input files for the inputs. The last class of options is also fixed in all of Gnuastro, it shows operating mode options. Most of these options are already explained in @ref{Operating modes}. @cindex Long outputs @cindex Redirection of output @cindex Command-line, long outputs The help message will sometimes be longer than the vertical size of your terminal. If you are using a graphical user interface terminal emulator, you can scroll the terminal with your mouse, but we promised no mice distractions! So here are some suggestions: @itemize @item @cindex Scroll command-line @cindex Command-line scroll @cindex @key{Shift + PageUP} and @key{Shift + PageDown} @key{Shift + PageUP} to scroll up and @key{Shift + PageDown} to scroll down. For most help output this should be enough. The problem is that it is limited by the number of lines that your terminal keeps in memory and that you can't scroll by lines, only by whole screens. @item @cindex Pipe @cindex @command{less} Pipe to @command{less}. A pipe is a form of shell re-direction. The @command{less} tool in Unix-like systems was made exactly for such outputs of any length. You can pipe (@command{|}) the output of any program that is longer than the screen to it and then you can scroll through (up and down) with its many tools. For example: @example $ astnoisechisel --help | less @end example @noindent Once you have gone through the text, you can quit @command{less} by pressing the @key{q} key. @item @cindex Save output to file @cindex Redirection of output Redirect to a file. This is a less convenient way, because you will then have to open the file in a text editor! You can do this with the shell redirection tool (@command{>}): @example $ astnoisechisel --help > filename.txt @end example @end itemize @cindex GNU Grep @cindex Searching text @cindex Command-line searching text In case you have a special keyword you are looking for in the help, you don't have to go through the full list. GNU Grep is made for this job. For example if you only want the list of options whose @option{--help} output contains the word ``axis'' in ImageCrop, you can run the following command: @example $ astimgcrop --help | grep axis @end example @cindex @code{ARGP_HELP_FMT} @cindex Argp argument parser @cindex Customize @option{--help} output @cindex @option{--help} output customization If the output of this option does not fit nicely within the confines of your terminal, GNU does enable you to customize its output through the environment variable @code{ARGP_HELP_FMT}, you can set various parameters which specify the formatting of the help messages. For example if your terminals are wider than 70 spaces (say 100) and you feel there is too much empty space between the long options and the short explanation, you can change these formats by giving values to this environment variable before running the program with the @option{--help} output. You can define this environment variable in this manner: @example $ export ARGP_HELP_FMT=rmargin=100,opt-doc-col=20 @end example @cindex @file{.bashrc} This will affect all GNU programs using GNU C library's @file{argp.h} facilities as long as the environment variable is in memory. You can see the full list of these formatting parameters in the ``Argp User Customization'' part of the GNU C library manual. If you are more comfortable to read the @option{--help} outputs of all GNU software in your customized format, you can add your customizations (similar to the line above, without the @command{$} sign) to your @file{~/.bashrc} file. This is a standard option for all GNU software. @node Man pages, Info, --help, Getting help @subsection Man pages @cindex Man pages Man pages were the Unix method of providing command-line documentation to a program. With GNU Info, see @ref{Info} the usage of this method of documentation is highly discouraged. This is because Info provides a much more easier to navigate and read environment. However, some operating systems require a man page for packages that are installed and some people are still used to this method of command line help. So the programs in Gnuastro also have Man pages which are automatically generated from the outputs of @option{--version} and @option{--help} using the GNU help2man program. So if you run @example $ man programname @end example @noindent You will be provided with a man page listing the options in the standard manner. @node Info, help-gnuastro mailing list, Man pages, Getting help @subsection Info @cindex GNU Info @cindex Command-line, viewing full book Info is the standard documentation format for all GNU software. It is a very useful command-line document viewing format, fully equipped with links between the various pages and menus and search capabilities. As explained before, the best thing about it is that it is available for you the moment you need to refresh your memory on any command-line tool in the middle of your work without having to take your hands off the keyboard. This complete book is available in Info format and can be accessed from anywhere on the command-line. To open the Info format of any installed programs or library on your system which has an Info format book, you can simply run the command below (change @command{executablename} to the executable name of the program or library): @example $ info executablename @end example @noindent @cindex Learning GNU Info @cindex GNU software documentation In case you are not already familiar with it, run @command{$ info info}. It does a fantastic job in explaining all its capabilities its self. It is very short and you will become sufficiently fluent in about half an hour. Since all GNU software documentation is also provided in Info, your whole GNU/Linux life will significantly improve. @cindex GNU Emacs @cindex GNU C library Once you've become an efficient navigator in Info, you can go to any part of this book or any other GNU software or library manual, no matter how long it is, in a matter of seconds. It also blends nicely with GNU Emacs (a text editor) and you can search manuals while you are writing your document or programs without taking your hands off the keyboard, this is most useful for libraries like the GNU C library. To be able to access all the Info manuals installed in your GNU/Linux within Emacs, type @key{Ctrl-H + i}. To see this whole book from the beginning in Info, you can run @example $ info gnuastro @end example @noindent If you run Info with the particular program executable name, for example @file{astimgcrop} or @file{astnoisechisel}: @example $ info astprogramname @end example @noindent you will be taken to the section titled ``Invoking ProgramName'' which explains the inputs and outputs along with the command-line options for that program. Finally, if you run Info with the official program name, for example ImageCrop or NoiseChisel: @example $ info ProgramName @end example @noindent you will be taken to the top section which introduces the program. Note that in all cases, Info is not case sensitive. @node help-gnuastro mailing list, , Info, Getting help @subsection help-gnuastro mailing list @cindex help-gnuastro mailing list @cindex Mailing list: help-gnuastro Gnuastro maintains the help-gnuastro mailing list for users to ask any questions related to Gnuastro. The experienced Gnuastro users and some of its developers are subscribed to this mailing list and your email will be sent to them immediately. However, when contacting this mailing list please have in mind that they are possibly very busy and might not be able to answer immediately. @cindex Mailing list archives @cindex @code{help-gnuastro@@gnu.org} To ask a question from this mailing list, send a mail to @code{help-gnuastro@@gnu.org}. Anyone can view the mailing list archives at @url{http://lists.gnu.org/archive/html/help-gnuastro/}. It is best that before sending a mail, you search the archives to see if anyone has asked a question similar to yours. If you want to make a suggestion or report a bug, please don't send a mail to this mailing list. We have other mailing lists and tools for those purposes, see @ref{Report a bug} or @ref{Suggest new feature}. @node Output headers, , Getting help, Common program behavior @section Output headers @cindex Output FITS headers @cindex CFITSIO version on outputs The output FITS files created by Gnuastro's programs have some or all of the following standard keywords to keep the basic date and version information of Gnuastro, its dependencies and the pipeline that is using Gnuastro. @table @command @item DATE The creation time of the FITS file. This date is written directly by CFITSIO and is in UT format. @item COMMIT Git's commit description from the running directory of Gnuastro's programs. If the running directory is not version controlled or @file{libgit2} isn't installed (see @ref{Optional dependencies}) then this keyword will not be present. The printed value is equivalent to the output of the following command: @example git describe --dirty --always @end example If the running directory contains non-committed work, then the stored value will have a `@command{-dirty}' suffix. This can be very helpful to let you know that the data is not ready to be shared with collaborators or submitted to a journal. You should only share results that are produced after all your work is committed (safely stored in the version controlled history and thus reproducible). At first sight, version control appears to be mainly a tool for software developers. However progress in a scientific research is almost identical to progress in software development: first you have a rough idea that starts with handful of easy steps. But as the first results appear to be promising, you will have to extend, or generalize, it to make it more robust and work in all the situations your research covers, not just your first test samples. Slowly you will find wrong assumptions or bad implementations that need to be fixed (`bugs' in software development parlance). Finally, when you submit the research to your collaborators or a journal, many comments and suggestions will come in, and you have to address them. Software developers have created version control systems precisely for this kind of activity. Each significant moment in the project's history is called a ``commit'', see @ref{Version controlled source}. A snapshot of the project in each ``commit'' is safely stored away, so you can revert back to it at a later time, or check changes/progress. This way, you can be sure that your work is reproducible and track the progress and history. With version control, experimentation in the project's analysis is greatly facilitated, since you can easily revert back if a brainstorm test procedure fails. One important feature of version control is that the research result (FITS image, table, report or paper) can be stamped with the unique commit information that produced it. This information will enable you to exactly reproduce that same result later, even if you have made changes/progress. For one example of a research paper's reproduction pipeline, please see the @url{https://gitlab.com/makhlaghi/NoiseChisel-paper, reproduction pipeline} of the @url{https://arxiv.org/abs/1505.01664, paper} describing @ref{NoiseChisel}. @item CFITSIO The version of CFITSIO used (see @ref{CFITSIO}). @item WCSLIB The version of WCSLIB used (see @ref{WCSLIB}). Note that older versions of WCSLIB do not report the version internally. So this is only available if you are using more recent WCSLIB versions. @item GNUASTRO The version of Gnuastro used (see @ref{Version numbering}). @end table Here is one example of the last few lines of an example output. @example / Versions and date DATE = '...' / file creation date COMMIT = 'v0-8-g547f6eb' / Commit description in running dir. CFITSIO = '3.39 ' / CFITSIO version. WCSLIB = '5.15 ' / WCSLIB version. GNUASTRO= '0.3' / GNU Astronomy Utilities version. END @end example @node Extensions and Tables, Image manipulation, Common program behavior, Top @chapter Extensions and Tables @cindex File operations @cindex Operations on files @cindex General file operations This chapter documents those Gnuastro programs that don't directly operate on the contents of the data file, they just print information, or convert from different data types. Before working on a FITS file, it is commonly the case that you are not sure how many extensions it has within it and also what each extension is (image, table or blank). In such cases, Header (see @ref{Header}) can be handy by printing the full header of a FITS file to the terminal for easy inspection. In other cases you want to use the data in a FITS file in other programs (for example in reports) that don't recognize the FITS format, for example converting a FITS image into a Jpeg, or PDF format image. ConvertType (see @ref{ConvertType}) was built for such situations. Finally, the FITS format is not just for images, it can also store tables. Binary tables in particular can be very useful in storing very large catalogs or tables compared to a plain text file. Table (see @ref{Table}) can be used to choose certain table columns in a FITS table and see them as a human readable output on the terminal, or to save them in another plain text or FITS table. @menu * Header:: Print and manipulate data file header. * ConvertType:: Convert data to various formats. * Table:: Read and Write FITS tables to plain text. @end menu @node Header, ConvertType, Extensions and Tables, Extensions and Tables @section Header The FITS standard requires each extension of a FITS file to have a header, giving basic information about what is in that extension. Each line in the header is for one keyword, specifying its name, value and a short comment string. Besides the basic information, the headers also contain vital information about the data, how they were processed, the instrument specifications that took the image and also the World Coordinate System that is used to translate pixel coordinates to sky or spectrum coordinates on the image or table. @menu * Invoking astheader:: Arguments and options to Header. @end menu @node Invoking astheader, , Header, Header @subsection Invoking Header Header can print or manipulate the header information in an extension of an astronomical data file. The executable name is @file{astheader} with the following general template @example $ astheader [OPTION...] ASTRdata @end example @noindent One line examples: @example $ astheader image.fits $ astheader --update=OLDKEY,153.034,"Old keyword comment" $ astheader --remove=COMMENT --comment="Anything you like ;-)." $ astheader --write=MYKEY1,20.00,"An example keyword" --write=MYKEY2,fd @end example @cindex HDU If no keyword modification options are given, the full header of the given HDU will be printed on the command-line. If any of the keywords are to be modified, the headers of the input file will be changed. If you want to keep the original FITS file, it is easiest to create a copy first and then run Header on that. In the FITS standard, keywords are always uppercase. So case does not matter in the input or output keyword names you specify. Most of the options can accept multiple instances in one command. For example you can add multiple keywords to delete by calling delete multiple times, since repeated keywords are allowed, you can even delete the same keyword multiple times. The action of such options will start from the top most keyword. @cartouche @noindent @strong{FITS STANDARD KEYWORDS:} Some header keywords are necessary for later operations on a FITS file, for example BITPIX or NAXIS, see the FITS standard for their full list. If you modify (for example remove or rename) such keywords, the FITS file extension might not be usable any more. Also be careful for the world coordinate system keywords, if you modify or change their values, any future world coordinate system (like RA and Dec) measurements on the image will also change. @end cartouche @cartouche @noindent @strong{PRECEDENCE:} The order of operations are as follows. Note that while the order within each class of actions is preserved, the order of individual actions is not. So irrespective of what order you called @option{--delete} and @option{--update}. First all the delete operations are going to take effect then the update operations. @enumerate @item @option{--delete} @item @option{--rename} @item @option{--update} @item @option{--write} @item @option{--asis} @item @option{--history} @item @option{--comment} @item @option{--date} @end enumerate @noindent All possible syntax errors will be reported before the keywords are actually written. FITS errors during any of these actions will be reported, but Header won't stop until all the operations are complete. If @option{quitonerror} is called, then Header will immediately stop upon the first error. @end cartouche @cindex GNU Grep If only a certain set of header keywords are desired, it is easiest to pipe the output of Header to GNU Grep. Grep is a very powerful and advanced tool to search strings which is precisely made for such situations. For example if you only want to check the size of an image FITS HDU, you can run: @example $ astheader input.fits | grep NAXIS @end example @noindent The options particular to Header can be seen below. See @ref{Common options} for a list of the options that are common to all Gnuastro programs, they are not repeated here. @table @option @item -a @itemx --asis (@option{=STR}) Write the string within this argument exactly into the FITS file header with no modifications. If it does not conform to the FITS standards, then it might cause trouble, so please be very careful with this option. If you want to define the keyword from scratch, it is best to use the @option{--write} option (see below) and let CFITSIO worry about the standards. The best way to use this option is when you want to add a keyword from one FITS file to another unchanged and untouched. Below is an example of such a case that can be very useful sometimes: @example $ key=$(astheader firstimage.fits | grep KEYWORD) $ astheader --asis="$key" secondimage.fits @end example @cindex GNU Bash In particular note the double quotation signs (@key{"}) around the reference to the @command{key} shell variable (@command{$key}), since FITS keywords usually have lots of space characters, if this variable is not enclosed within double quotation marks, the shell will only give the first word in the full keyword to this option, which will definitely be a non-standard FITS keyword and will make it hard to work on the file afterwords. See the ``Quoting'' section of the GNU Bash manual for more information if your keyword has the special characters @key{$}, @key{`}, or @key{\}. @item -d @itemx --delete (@option{=STR}) Delete one instance of the desired keyword. Multiple instances of @option{--delete} can be given (possibly even for the same keyword). All keywords given will be removed from the headers in the opposite order (last given keyword will be deleted first). If the keyword doesn't exist, Header will give a warning and return with a non-zero value, but will not stop. @item -r @itemx --rename (@option{=STR}) Rename a keyword to a new value. The old name and the new name should be separated by either a comma (@key{,}) or a space character. Note that if you use a space character, you have to put the value to this option within double quotation marks (@key{"}) so the space character is not interpreted as an option separator. Multiple instances of @option{--rename} can be given in one command. The keywords will be renamed in the specified order. @item -u @itemx --update (@option{=STR}) Update a keyword, its value, its comments and its units all defined separately. If there are multiple instances of the keyword in the header, they will be changed from top to bottom (with multiple @option{--update} options). @noindent The format of the values to this option can best be specified with an example: @example --update=KEYWORD,value,"comments for this keyword",unit @end example @noindent The value can be any numerical or string value@footnote{Some tricky situations arise with values like `@command{87095e5}', if this was intended to be a number it will be kept in the header as @code{8709500000} and there is no problem. But this can also be a shortened Git commit hash. In the latter case, it should be treated as a string and stored as it is written. Commit hashes are very important in keeping the history of a file during your research and such values might arise without you noticing them in your reproduction pipeline. One solution is to use @command{git describe} instead of the short hash alone. A less recommended solution is to add a space after the commit hash and Header will write the value as `@command{87095e5 }' in the header. If you later compare the strings on the shell, the space character will be ignored by the shell in the latter solution and there will be no problem.}. Other than the @code{KEYWORD}, all the other values are optional. To leave a given token empty, follow the preceding comma (@key{,}) immediately with the next. If any space character is present around the commas, it will be considered part of the respective token. So if more than one token has space characters within it, the safest method to specify a value to this option is to put double quotation marks around each individual token that needs it. Note that without double quotation marks, space characters will be seen as option separators and can lead to undefined behavior. @item -w @itemx --write (@option{=STR}) Write a keyword to the header. For the possible value input formats, comments and units for the keyword, see the @option{--update} option above. @item -H @itemx --history (@option{=STR}) Add a @code{HISTORY} keyword to the header. The string given to this keyword will be separated into multiple keyword cards if it is longer than 70 characters. With each run only one value for the @option{--history} option will be read. If there are multiple, it is the last one. @item -c @itemx --comment (@option{=STR}) Add a @code{COMMENT} keyword to the header. Similar to the explanation for @option{--history} above. @item -t @itemx --date Put the current date and time in the header. If the @code{DATE} keyword already exists in the header, it will be updated. @item -Q @itemx --quitonerror Quit if any of the operations above are not successful. By default if an error occurs, Header will warn the user of the faulty keyword and continue with the rest of actions. @end table @node ConvertType, Table, Header, Extensions and Tables @section ConvertType @cindex Data format conversion @cindex Converting data formats @cindex Image format conversion @cindex Converting image formats @pindex @r{ConvertType (}astconvertt@r{)} The formats of astronomical data were defined mainly for archiving and processing. In other situations, the data might be useful in other formats. For example, when you are writing a paper or report or if you are making slides for a talk, you can't use a FITS image. Other image formats should be used. In other cases you might want your pixel values in a table format as plain text for input to other programs that don't recognize FITS, or to include as a table in your report. ConvertType is created for such situations. The various types will increase with future updates and based on need. The conversion is not only one way (from FITS to other formats), but two ways (except the EPS and PDF formats). So you can convert a JPEG image or text file into a FITS image. Basically, other than EPS, you can use any of the recognized formats as different color channel inputs to get any of the recognized outputs. So before explaining the options and arguments, first a short description of the recognized files types will be given followed a short introduction to digital color. @menu * Recognized file types:: Recognized file types * Color:: Some explanations on color. * Invoking astconvertt:: Options and arguments to ConvertType. @end menu @node Recognized file types, Color, ConvertType, ConvertType @subsection Recognized file types The various standards and the file name extensions recognized by ConvertType are listed below. @table @asis @item FITS or IMH @cindex Astronomical data format Astronomical data are commonly stored in the FITS format (and in older data sets in IRAF @file{.imh} format), a list of file name suffixes which indicate that the file is in this format is given in @ref{Arguments}. Each extension of a FITS image only has one value per pixel, so when used as input, each input FITS image contributes as one color channel. If you want multiple extensions in one FITS file for different color channels, you have to repeat the file name multiple times and use the @option{--hdu}, @option{--hdu2}, @option{--hdu3} or @option{--hdu4} options to specify the different extensions. @item JPEG @cindex JPEG format @cindex Raster graphics @cindex Pixelated graphics The JPEG standard was created by the Joint photographic experts group. It is currently one of the most commonly used image formats. Its major advantage is the compression algorithm that is defined by the standard. Like the FITS standard, this is a raster graphics format, which means that it is pixelated. A JPEG file can have 1 (for grayscale), 3 (for RGB) and 4 (for CMYK) color channels. If you only want to convert one JPEG image into other formats, there is no problem, however, if you want to use it in combination with other input files, make sure that the final number of color channels does not exceed four. If it does, then ConvertType will abort and notify you. @cindex Suffixes, JPEG images The file name endings that are recognized as a JPEG file for input are: @file{.jpg}, @file{.JPG}, @file{.jpeg}, @file{.JPEG}, @file{.jpe}, @file{.jif}, @file{.jfif} and @file{.jfi}. @item EPS @cindex EPS @cindex PostScript @cindex Vector graphics @cindex Encapsulated PostScript The Encapsulated PostScript (EPS) format is essentially a one page PostScript file which has a specified size. PostScript also includes non-image data, for example lines and texts. It is a fully functional programming language to describe a document. Therefore in ConvertType, EPS is only an output format and cannot be used as input. Contrary to the FITS or JPEG formats, PostScript is not a raster format, but is categorized as vector graphics. @cindex PDF @cindex Adobe systems @cindex PostScript vs. PDF @cindex Compiled PostScript @cindex Portable Document format @cindex Static document description format The Portable Document Format (PDF) is currently the most common format for documents. Some believe that PDF has replaced PostScript and that PostScript is now obsolete. This view is wrong, a PostScript file is an actual plain text file that can be edited like any program source with any text editor. To be able to display its programmed content or print, it needs to pass through a processor or compiler. A PDF file can be thought of as the processed output of the compiler on an input PostScript file. PostScript, EPS and PDF were created and are registered by Adobe Systems. @cindex @TeX{} @cindex @LaTeX{} With these features in mind, you can see that when you are compiling a document with @TeX{} or @LaTeX{}, using an EPS file is much more low level than a JPEG and thus you have much greater control and therefore quality. Since it also includes vector graphic lines we also use such lines to make a thin border around the image to make its appearance in the document much better. No matter the resolution of the display or printer, these lines will always be clear and not pixelated. In the future, addition of text might be included (for example labels or object IDs) on the EPS output. However, this can be done better with tools within @TeX{} or @LaTeX{} such as PGF/Tikz@footnote{@url{http://sourceforge.net/projects/pgf/}}. @cindex Binary image @cindex Saving binary image @cindex Black and white image If the final input image (possibly after all operations on the flux explained below) is a binary image or only has two colors of black and white (in segmentation maps for example), then PostScript has another great advantage compared to other formats. It allows for 1 bit pixels (pixels with a value of 0 or 1), this can decrease the output file size by 8 times. So if a grayscale image is binary, ConvertType will exploit this property in the EPS and PDF (see below) outputs. @cindex Suffixes, EPS format The standard formats for an EPS file are @file{.eps}, @file{.EPS}, @file{.epsf} and @file{.epsi}. The EPS outputs of ConvertType have the @file{.eps} suffix. @item PDF @cindex Suffixes, PDF format @cindex GPL Ghostscript As explained above, a PDF document is a static document description format, viewing its result is therefore much faster and more efficient than PostScript. To create a PDF output, ConvertType will make a PostScript page description and convert that to PDF using GPL Ghostscript. The suffixes recognized for a PDF file are: @file{.pdf}, @file{.PDF}. If GPL Ghostscript cannot be run on the PostScript file, it will remain and a warning will be printed. @item @option{blank} @cindex @file{blank} color channel This is not actually a file type! But can be used to fill one color channel with a blank value. If this argument is given for any color channel, that channel will not be used in the output. @item Plain text @cindex Plain text @cindex Suffixes, plain text Plain text files have the advantage that they can be viewed with any text editor or on the command-line. Most programs also support input as plain text files. In ConvertType, if the input arguments do not have any of the extensions listed above for other formats, the input is assumed to be a text file. Each plain text file is considered to contain one color channel. There is no standard output for plain text files. @cindex Mis-spelling file suffix @cindex File suffix mis-spelling If any of the extension above is mis-spelled, this will result in the output becoming a plain text file with that (short) name. If this happens, ConvertType will warn you and write the output as a plain text file. If you don't want that warning, set your plain text output file names longer than 5 characters. When converting an image to plain text, consider the fact that if the image is large the number of columns in each line will become very large, possibly making it very hard to open in some text editors. @end table @node Color, Invoking astconvertt, Recognized file types, ConvertType @subsection Color @cindex RGB @cindex CMYK @cindex Image @cindex Pixels @cindex Grayscale @cindex Colorspace @cindex Primary colors @cindex Colorspace, grayscale An image is a two dimensional array of 2 dimensional elements called pixels. If each pixel only has one value, the image is known as a grayscale image and no color is defined. The range of values in the image can be interpreted as shades of any color, it is customary to use shades of black or grayscale. However, to produce the color spectrum in the digital world, several primary colors must be mixed. Therefore in a color image, each pixel has several values depending on how many primary colors were chosen. For example on the digital monitor or color digital cameras, all colors are built by mixing the three colors of Red-Green-Blue (RGB) with various proportions. However, for printing on paper, standard printers use the Cyan-Magenta-Yellow-Key (CMYK, Key=black) color space. Therefore when printing an RGB image, usually a transformation of color spaces will be necessary. In a colored digital camera, a color image is produced by dividing the pixel's area between three colors (filters). However in astronomy due to the intrinsic faintness of most of the targets, the collecting area of the pixel is very important for us. Hence the full area of the pixel is used and one value is stored for that pixel in the end. One color filter is used for the whole image. Thus a FITS image is inherently a grayscale image and no color can be defined for it. @cindex Colorspace, transformation One way to represent a grayscale image in different color spaces is to use the same proportions of the primary colors in each pixel. This is the common way most FITS image converters work: they fill all the channels with the same values. The downside is two fold: @itemize @item Three (for RGB) or four (for CMYK) values have to be stored for every pixel, this makes the output file very heavy (in terms of bytes). @item If printing, the printing errors of each color channel can make the printed image slightly more blurred than it actually is. @end itemize @cindex PNG standard @cindex Single channel CMYK To solve both these problems, the best way is to save the FITS image into the black channel of the CMYK color space. In the RGB color space all three channels have to be used. The JPEG standard is the only common standard that accepts CMYK color space, that is why currently only the JPEG standard is included and not the PNG standard for example. The JPEG and EPS standards set two sizes for the number of bits in each channel: 8-bit and 12-bit. The former is by far the most common and is what is used in ConvertType. Therefore, each channel should have values between 0 to @math{2^8-1=255}. From this we see how each pixel in a grayscale image is one byte (8 bits) long, in an RGB image, it is 3bytes long and in CMYK it is 4bytes long. But thanks to the JPEG compression algorithms, when all the pixels of one channel have the same value, that channel is compressed to one pixel. Therefore a Grayscale image and a CMYK image that has only the K-channel filled are approximately the same file size. @node Invoking astconvertt, , Color, ConvertType @subsection Invoking ConvertType ConvertType will convert any recognized input file type to any specified output type. The executable name is @file{astconvertt} with the following general template @example $ astconvertt [OPTION...] InputFile [InputFile2] ... [InputFile4] @end example @noindent One line examples: @example $ astconvertt M31.fits --output=pdf $ astconvertt galaxy.jpg -ogalaxy.fits $ astconvertt f1.txt f2.txt f3.fits -o.jpg $ astconvertt M31_r.fits M31_g.fits blank -oeps @end example @noindent The file type of the output will be specified with the (possibly complete) file name given to the @option{--output} option, which can either be given on the command-line or in any of the configuration files (see @ref{Configuration files}). Note that if the output suffix is not recognized, it will default to plain text format, see @ref{Recognized file types}. The order of multiple input files is important. After reading the input file(s) the number of color channels in all the inputs will be used to define which color space is being used for the outputs and how each color channel is interpreted. Note that one file might have more than one color channel (for example in the JPEG format). If there is one color channel the output is grayscale, if three input color channels are given they are respectively considered to be the red, green and blue color channels and if there are four color channels they are respectively considered to be cyan, magenta, yellow and black. The value to @option{--output} (or @option{-o}) can be either a full file name or just the suffix of the desired output format. In the former case, that same name will be used for the output. In the latter case, the name of the output file will be set based on the automatic output guidelines, see @ref{Automatic output}. Note that the suffix name can optionally start a @file{.} (dot), so for example @option{--output=.jpg} and @option{--output=jpg} are equivalent. Be careful that if you want your output in plain text, you have to give the full file name. So if @option{-otxt} or @option{--output=.txt} are given, the output file will be named @file{txt} or @file{.txt} (the latter will be a hidden file!). Besides the common set of options explained in @ref{Common options}, the options to ConvertType can be classified into input, output and flux related options. The majority of the options are to do with the flux range. Astronomical data usually have a very large dynamic range (difference between maximum and minimum value) and different subjects might be better demonstrated with a limited flux range. @noindent Input: @table @option @item --hdu2 If the second input file is a FITS file, the value to this option will be used to specify which HDU will be used. Note that for the first file, the (@option{--hdu} or @option{-h} in the common options is used) @item --hdu3 The HDU of the third input FITS file. @item --hdu4 The HDU of the fourth input FITS file. @end table @noindent Output: @table @option @item -w @itemx --widthincm (@option{=FLT}) The width of the output in centimeters. This is only relevant for those formats that accept such a width (not plain text for example). For most digital purposes, the number of pixels is far more important than the value to this parameter because you can adjust the absolute width (in inches or centimeters) in your document preparation program. @item -b @itemx --borderwidth @cindex Border on an image (@option{=INT}) The width of the border to be put around the EPS and PDF outputs in units of PostScript points. There are 72 or 28.35 PostScript points in an inch or centimeter respectively. In other words, there are roughly 3 PostScript points in every millimeter. If you are planning on adding a border, its significance is highly correlated with the value you give to the @option{--widthincm} parameter. Unfortunately in the document structuring convention of the PostScript language, the ``bounding box'' has to be in units of PostScript points with no fractions allowed. So the border values only have to be specified in integers. To have a final border that is thinner than one PostScript point in your document, you can ask for a larger width in ConvertType and then scale down the output EPS or PDF file in your document preparation program. For example by setting @command{width} in your @command{includegraphics} command in @TeX{} or @LaTeX{}. Since it is vector graphics, the changes of size have no effect on the quality of your output quality (pixels don't get different values). @item -x @itemx --hex @cindex ASCII85 encoding @cindex Hexadecimal encoding Use Hexadecimal encoding in creating EPS output. By default the ASCII85 encoding is used which provides a much better compression ratio. When converted to PDF (or included in @TeX{} or @LaTeX{} which is finally saved as a PDF file), an efficient binary encoding is used which is far more efficient than both of them. The choice of EPS encoding will thus have no effect on the final PDF. So if you want to transfer your EPS files (for example if you want to submit your paper to arXiv or journals in PostScript), their storage might become important if you have large images or lots of small ones. By default ASCII85 encoding is used which offers a much better compression ratio (nearly 40 percent) compared to Hexadecimal encoding. @item -u @itemx --quality @cindex JPEG compression quality @cindex Compression quality in JPEG @cindex Quality of compression in JPEG (@option{=INT}) The quality (compression) of the output JPEG file with values from 0 to 100 (inclusive). For other formats the value to this option is ignored. Note that only in grayscale (when one input color channel is given) will this actually be the exact quality (each pixel will correspond to one input value). If it is in color mode, some degradation will occur. While the JPEG standard does support loss-less graphics, it is not commonly supported. @end table @noindent Flux range: @table @option @item -c @itemx --change @cindex Change converted pixel values (@option{=STR}) Change pixel values with the following format @option{"from1:to1, from2:to2,..."}. This option is very useful in displaying labeled pixels (not actual data images which have noise) like segmentation maps. In labeled images, usually a group of pixels have a fixed integer value. With this option, you can manipulate the labels before the image is displayed to get a better output for print or to emphasize on a particular set of labels and ignore the rest. The labels in the images will be changed in the same order given. By default first the pixel values will be converted then the pixel values will be truncated (see @option{--fluxlow} and @option{--fluxhigh}). You can use any number for the values irrespective of your final output, your given values are stored and used in the double precision floating point format. So for example if your input image has labels from 1 to 20000 and you only want to display those with labels 957 and 11342 then you can run ConvertType with these options: @example $ astconvertt --change=957:50000,11342:50001 --fluxlow=5e4 \ --fluxhigh=1e5 segmentationmap.fits --output=jpg @end example @noindent While the output JPEG format is only 8 bit, this operation is done in an intermediate step which is stored in double precision floating point. The pixel values are converted to 8-bit after all operations on the input fluxes have been complete. By placing the value in double quotes you can use as many spaces as you like for better readability. @item -C @itemx --changeaftertrunc Change pixel values (with @option{--change}) after truncation of the flux values, by default it is the opposite. @item -L @itemx --fluxlow (@option{=FLT}) The minimum flux (pixel value) to display in the output image, any pixel value below this value will be set to this value in the output. If the value to this option is the same as @option{--fluxmax}, then no flux truncation will be applied. Note that when multiple channels are given, this value is used for all the color channels. @item -H @itemx --fluxhigh (@option{=FLT}) The maximum flux (pixel value) to display in the output image, see @option{--fluxlow}. @item -m @itemx --maxbyte (@option{=INT}) This is only used for the JPEG and EPS output formats which have an 8-bit space for each channel of each pixel. The maximum value in each pixel can therefore be @mymath{2^8-1=255}. With this option you can change (decrease) the maximum value. By doing so you will decrease the dynamic range. It can be useful if you plan to use those values for other purposes. @item -i @itemx --flminbyte (@option{=INT}) If the lowest pixel value in the input channels is larger than the value to @option{--fluxlow}, then that input value will be redundant. In some situations it might be necessary to set the minimum byte value (0) to correspond to that flux even if the data do not reach that value. With this option you can do this. Note that if the minimum pixel value is smaller than @option{--fluxlow}, then this option is redundant. @item -a @itemx --fhmaxbyte (@option{=INT}) See @option{--flminbyte}. @item -l @itemx --log Display the logarithm of the input data. This is done after the conversion and flux truncation steps, see above. @item -n @itemx --noinvert For 8-bit output types (JPEG and EPS for example) the final value that is stored is inverted so white becomes black and vice versa. The reason for this is that astronomical images usually have a very large area of blank sky in them. The result will be that a large are of the image will be black. Therefore, by default the 8-bit values are inverted so the images blend in better with the text in a document. Note that this behaviour is ideal for grayscale images, if you want a color image, the colors are going to be mixed up. For color images it is best to call this option so the image is not inverted. @end table @node Table, , ConvertType, Extensions and Tables @section Table The FITS standard is not just for storing astronomical images, from its early days, it also included tables. Tables are the products of processing astronomical images and spectra. For example in Gnuastro, MakeCatalog will process the defined pixels over an object and produce a catalog (see @ref{MakeCatalog}). For each identified object, MakeCatalog can print its position on the image or sky, its total brightness and many other information that is deducible from the given image. Each one of these properties is a column in its output catalog (or table) and for each input object, we have a row. When there are only a small number of objects (rows) and not too many properties (columns), then a simple plain text file is mainly enough to store, transfer, or even use the produced data. However, to be more efficient in all these aspects, astronomers have defined the FITS binary table standard to store data in a binary (0 and 1) format, not plain text. This can offer major advantages in all those aspects: the file size will be greatly reduced and the reading and writing will be faster (because the RAM and CPU also work in binary). The FITS standard also defines a standard for ASCII tables, where the data are stored in the human readable ASCII format, but within the FITS file structure. These are mainly useful for keeping ASCII data along with images and possibly binary data as multiple (conceptually related) extensions within a FITS file. @cindex AWK @cindex GNU AWK However, this comes at a cost: binary tables are not easily readable by human eyes. There is no standard on how the zero and ones should be interpretted. The Unix-like operating systems have flourished because of a simple fact: communication between the various tools is based on human readable characters@footnote{In ``The art of Unix programming'', Eric Raymond makes this suggestion to programmers: ``When you feel the urge to design a complex binary file format, or a complex binary application protocol, it is generally wise to lie down until the feeling passes.''. This is a great book and strongly recommended, give it a look if you want to truly enjoy your work/life in this environment.}. So while the FITS table standards are very beneficial for the tools that recognize them, they are hard to use in the vast majority of available software. This creates limitations for their generic use. `Table' is Gnuastro's solution to this problem. With Table, FITS tables (ASCII or binary) are directly accessible to the Unix-like operating systems power-users (those working the command-line or shell, see @ref{Command-line interface}). With Table, a FITS table (in binary or ASCII formats) is only one command away from AWK (or any other tool you want to use). Just like a plain text file that you read with the @command{cat} command. You can pipe the output of Table into any other tool for higher-level processing, see the examples in @ref{Invoking asttable} for some very simple examples. @menu * Invoking asttable:: Options and arguments to Table. @end menu @node Invoking asttable, , Table, Table @subsection Invoking Table Table will convert FITS binary and ASCII tables into other such tables, or print them on the command-line, or save them in a plain text file. Output columns can also be determined by number or regular expression matching of column names. The executable name is @file{asttable} with the following general template @example $ asttable [OPTION...] InputFile @end example @noindent One line examples: @example ## Get the table column information (name, data type, or units) $ asttable bintab.fits --information ## Only print those columns which have a name starting with "MAG_" $ asttable bintab.fits --columns=^MAG_ ## Only print the 2nd column, and the third column multiplied by 5 $ asttable bintab.fits | awk '@{print $2, 5*$3@}' ## Only print those rows with a value in the 10th column above 100000 $ asttable bintab.fits | awk '$10>10e5 @{print@}' ## Sort the output columns by the third column, save output $ asttable bintab.fits | sort -k3 > output.txt ## Convert a plain text table to a binary FITS table $ asttable plaintext.txt --output=inbinary.fits @end example Table can accept plain text files, or binary and ASCII FITS table extensions in a FITS file. For the full list of options common to all Gnuastro utilities please see @ref{Common options}. Options can also be stored in directory, user or system-wide configuration files to avoid repeating on the command-line, see @ref{Configuration files}. Currently all plain text files are processed (and thus printed, or saved to a binary FITS table) as double floating point types. We are still working on this many many more features. Table does not follow Automatic output that is common in most Gnuastro, see @ref{Automatic output}. If no value is given to the @option{--output} option, the desired columns will be printed to the standard output (on the command-line). This feature makes it very useful to directly pipe the output as input to other programs as the examples above demonstrate. Note that the options below which relate to print formatting are only relevant when the output is in human readable format (on the command-line and plain text files), they are ignored when the output is a binary FITS table. @table @option @item -i @itemx --information Print the information for each column and abort. The information for each column will be printed as a row on the command-line. The column name (if present), units (if present) and datatype will printed. Note that the FITS standard does not require a name or units for columns, only the datatype is mandatory. @item -c @itemx --column (@option{=STR} or @option{=INT}) Specify the columns to output for this table. If an integer number is given, the column number will be used (counting from 1). Otherwise the value (a string) will be passed to an internal regular expression processor which will try to match all the columns in the table with the given regular expression. Currently only FITS tables might have column names (it is an optional feature in the FITS standard). There is currently no particular standard to name plain text columns. This option can be called any number of times with one run of Table. The order of the output columns will be determined by the input order. This option is also not mandatory. If not given, all the input table columns are output. Regular expressions are a very powerful tool in matching text and since FITS binary tables usually have a large number of columns, this feature can greatly simply the selection of the output columns. @item -I @itemx --ignorescase Ignore case while matching the column names with the value(s) of the @option{--column} option. The FITS standard suggests to treat the column names as case insensitive, however it is not a requirement. @item --feg (@option{=STR}) Format of printing floating point numbers in non-binary outputs. It can only accept one of the three following values (same as C's @code{printf}): @itemize @item @key{f}: Print complete floating point value, this is good when the numbers aren't too small, for example @mymath{3.286}. But it will print all the zeros in @mymath{3.2\times10^{-15}}. @item @key{e}: Only print in exponential format. This is good for very large or very small numbers, but can make reading the values of more ordinary numbers a little hard. @item @key{g}: Let the system choose which representation is better for the number. @end itemize @item --sintwidth (@option{=INT}) The minimum width (number of characters) for printing columns of shorter integer datatypes. The shorter datatypes are considered to be signed and unsigned characters, short integers, integers. @item --lintwidth (@option{=INT}) The minimum width (number of characters) for printing columns of longer datatypes. The longer datatypes are considered to be @code{long} and @code{longlong} types. @item --floatwidth (@option{=INT}) The minimum width (number of characters) for printing columns of single precision floating point datatypes. @item --doublewidth (@option{=INT}) The minimum width (number of characters) for printing columns of double precision floating point datatypes. @item --strwidth (@option{=INT}) The minimum width (number of characters) for printing columns of strings (given as one column, the FITS standard allows ASCII strings as table elements). @item --floatprecision (@option{=INT}) The number of digits to print after the floating point for single precision floating point numbers. @item --doubleprecision (@option{=INT}) The number of digits to print after the floating point for double precision floating point numbers. @item --fitstabletype (@option{=STR}) The type of FITS table when a FITS file is specified as the output. This option can only have two values: @option{binary}, or @option{ascii}. However, currently ASCII FITS table outputs are not yet implemented due to lack of need. If you need it, please get in touch with so we implement it. @end table @node Image manipulation, Image analysis, Extensions and Tables, Top @chapter Image manipulation Images are one of the major formats of data that is used in astronomy. The functions in this chapter explain the GNU Astronomy Utilities which are provided for their manipulation. For example cropping out a part of a larger image or convolving the image with a given kernel or applying a transformation to it. @menu * ImageCrop:: Crop region(s) from FITS image(s). * Arithmetic:: Arithmetic on input data. * Convolve:: Convolve an image with a kernel. * ImageWarp:: Warp/Transform an image to a different grid. * SubtractSky:: Find the sky and subtract it from image. @end menu @node ImageCrop, Arithmetic, Image manipulation, Image manipulation @section ImageCrop @cindex Section of an image @cindex Crop part of image @cindex Postage stamp images @cindex Large astronomical images @pindex @r{ImageCrop (}astimgcrop@r{)} Astronomical images are often very large, filled with thousands of galaxies. It often happens that you only want a section of the image, or you have a catalog of sources and you want to visually analyze them in small postage stamps. ImageCrop is made to do all these things. When more than one crop is required, ImageCrop will divide the crops between multiple threads to significantly reduce the run time. @cindex Mosaicing @cindex Image tiles @cindex Image mosaic @cindex COSMOS survey @cindex Imaging surveys @cindex Hubble Space Telescope Astronomical surveys are usually extremely large. So large in fact, that the whole survey will not fit into a reasonably sized file. Because of this surveys usually cut the final image into separate tiles and store each tile in a file. For example the COSMOS survey's Hubble space telescope, ACS F814W image consists of 81 separate FITS images, with each one having a volume of 1.7 Giga bytes. @cindex Stitch multiple images Even though the tile sizes are chosen to be large enough that too many galaxies don't fall on the edges of the tiles, inevitably some do and if you simply crop the image of the galaxy from that one tile, you will miss a large area of the surrounding sky (which is essential in estimating the noise). Therefore in its WCS mode, ImageCrop will stitch parts of the tiles that are relevant for a target (with the given width) from all the input images that cover that region into the output. Of course, the tiles have to be present in the list of input files. ImageCrop also has facilities to crop arbitrary polygons from a set of tiles by stitching the relevant parts of different tiles within the polygon, see @option{--polygon} in @ref{Invoking astimgcrop}. Alternatively, it can crop out rectangular regions from one image which can come in handy when removing the bias pixels in raw image processing, see @ref{Crop section syntax}. @menu * ImageCrop modes:: Basic ImageCrop modes. * Crop section syntax:: How to define a section to crop. * Blank pixels:: Pixels with no value. * Invoking astimgcrop:: Calling ImageCrop on the command-line @end menu @node ImageCrop modes, Crop section syntax, ImageCrop, ImageCrop @subsection ImageCrop modes In order to be as comprehensive as possible, ImageCrop has two major modes of operation listed below. @table @asis @item Image The image mode uses the pixel coordinates. Depending on your command line options, this mode consists of three sub-modes. In image mode, only one image may be input. @itemize @item Catalog (multiple crops). Coordinates are read from a text file. The @option{--xcol} and @option{--ycol} columns in the catalog are interpreted as the center of a square crop box whose width is specified with the @option{--iwidth} option in pixels. Since the given pixel has to be on the center, the width has to be an odd number, so if you give an even number for the width, it will be added by one. If a catalog file name is provided (with @option{--imagemode} activated of course) this mode will be used. @item Center (one crop). The box center is given on the command-line with the @option{--xc} and @option{--yc} parameters. The image width is similar to above. @item Section (one crop). You can specify the section of pixels along each axis in the image which you want to be cropped with the @option{--section} option. See @ref{Crop section syntax} for a full explanation on the syntax of specifying the desired region. @end itemize The latter two cases will only have one crop box. In both cases, ImageCrop will go into the image mode, irrespective of calling @option{--wcsmode} or the default mode. In the first two cases, since you specify a central pixel, the crop box will be a square with an odd number of pixels on the side, so your desired pixel sits right in the center, see @ref{Blank pixels} on how to disable this for cases when the box exceeds the image size. @item WCS The Right ascension (RA) and Declination (Dec) of the objects in a catalog is used to define the central position of each postage stamp. In this mode, the width (@option{--wwidth}) is read in units of arc seconds and multiple images (tiles in a survey) can be input. If the objects are closer to the edge of the image than half the required width, other tiles (if they are present in the input files) are used to fill the empty space. The square output cropped box will have an odd number of pixels on the side. In this mode, the input images do not necessarily have to be the same size, each individual tile can even be smaller than the final crop. In any case, any part of any of the input images which overlaps with the desired region will be used in the crop. Note that if there is an over lap, the pixels from the last input image read are going to be used. The input images all just have to be aligned with the celestial coordinates, see the caution note below. Similar to the image mode, there are two sub-modes: @itemize @item Catalog (multiple crops). Similar to catalog mode in image mode. The RA and Dec column should be specified in the catalog (@option{--racol} and @option{--deccol}). @item Center (one crop). You can specify the center of only one crop box (no matter how many input images there are) with the options @option{--ra} and @option{--dec}. If it exists in the input images, it will be cropped similar to the catalog mode. If automatic output is triggered (you don't specify a file name for @option{--output}) and several of the input images are used to stitch and crop the region around the central point, the name of the first input will be used in automatic output, see @ref{Automatic output}. @end itemize @cartouche @noindent @strong{CAUTION:} In WCS mode, the image has to be aligned with the celestial coordinates, such that the first FITS axis is parallel (opposite direction) to the Right Ascension (RA) while the second FITS axis is parallel to the declination. If these conditions aren't met for an image, ImageCrop will warn you and abort. You have to use other tools to transform the image to the correct directions. @end cartouche @end table In short, if you don't specify a catalog, you have to specify box coordinates manually on the command-line. When you do specify a catalog, ImageCrop has to be in one of the two major modes (@option{--imgmode} or @option{--wcsmode}). Note that the single crop box parameters specified in the sub-modes will not be written to or read from the configuration file, they have to be specified on each execution. @node Crop section syntax, Blank pixels, ImageCrop modes, ImageCrop @subsection Crop section syntax @cindex Crop a given section of image When in image mode, one of the methods to crop only one rectangular section from the input image is to use the @option{--section} option. ImageCrop has a powerful syntax to read the box parameters from a string of characters. If you leave certain parts of the string to be empty, ImageCrop can fill them for you based on the input image sizes. @cindex Define section to crop To define a box, you need the coordinates of two points: the first pixel in the box at (@code{X1}, @code{Y1}) and the pixel which is immediately outside of the box (@code{X2, @code{Y2}}), four coordinates in total. The four coordinates can be specified with one string in this format: @command{X1:X2,Y1:Y2}. It is given to the @option{--section} option. Therefore, the pixels along the first axis that are @math{\geq}@command{X1} and <@command{X2} will be included in the cropped image. The same goes for the second axis. Note that each different term will be read as an integer, not a float (there are no sub-pixels in ImageCrop, you can use ImageWarp to shift the matrix with any sub-pixel distance, then crop the warped image, see @ref{ImageWarp}). Also, following the FITS standard, pixel indexes along each axis start from unity(1) not zero(0). @cindex Crop section format You can omit any of the values and they will be filled automatically. The left hand side of the colon (@command{:}) will be filled with @command{1}, and the right side with the image size. So, @command{2:,:} will include the full range of pixels along the second axis and only those with a first axis index larger than @command{2} in the first axis. If the colon is omitted for a dimension, then the full range is automatically used. So the same string is also equal to @command{2:,} or @command{2:} or even @command{2}. If you want such a case for the second axis, you should set it to: @command{,2}. If you specify a negative value, it will be seen as before the indexes of the image which are outside the image along the bottom or left sides when viewed in SAO ds9. In case you want to count from the top or right sides of the image, you can use an asterisk (@option{*}). When confronted with a @option{*}, ImageCrop will replace it with the maximum length of the image in that dimension. So @command{*-10:*+10,*-20:*+20} will mean that the crop box will be @math{20\times40} pixels in size and only include the top corner of the input image with 3/4 of the image being covered by blank pixels, see @ref{Blank pixels}. If you feel more comfortable with space characters between the values, you can use as many space characters as you wish, just be careful to put your value in double quotes, for example @command{--section="5:200, 123:854"}. If you forget, anything after the first space will not be seen by @option{--section}, because the unquoted space character is one of the characters that separates options on the command-line. @node Blank pixels, Invoking astimgcrop, Crop section syntax, ImageCrop @subsection Blank pixels @cindex Blank pixel The cropped box can potentially include pixels that are beyond the image range. For example when a target in the input catalog was very near the edge of the input image. The parts of the cropped image that were not in the input image will be filled with the following two values depending on the data type of the image. In both cases, SAO ds9 will not color code those pixels. @itemize @item If the data type of the image is a floating point type (float or double), IEEE NaN (Not a number) will be used. @item For integer types, pixels out of the image will be filled with the value of the @command{BLANK} keyword in the cropped image header. The value assigned to it is the lowest value possible for that type, so you will probably never need it any way. Only for the unsigned character type (@command{BITPIX=8} in the FITS header), the maximum value is used because it is unsigned, the smallest value is zero which is often meaningful. @end itemize You can ask for such blank regions to not be included in the output crop image using the @option{--noblank} option. In such cases, there is no guarantee that the image size of your outputs are what you asked for. In some survey images, unfortunately they do not use the @command{BLANK} FITS keyword. Instead they just give all pixels outside of the survey area a value of zero. So by default, when dealing with float or double image types, any values that are 0.0 are also regarded as blank regions. This can be turned off with the @option{--zeroisnotblank} option. @node Invoking astimgcrop, , Blank pixels, ImageCrop @subsection Invoking ImageCrop ImageCrop will crop a region from an image. If in WCS mode, it will also stitch parts from separate images in the input files. The executable name is @file{astimgcrop} with the following general template @example $ astimgcrop [OPTION...] [ASCIIcatalog] ASTRdata ... @end example @noindent One line examples: @example $ astimgcrop -I catalog.txt image.fits $ astimgcrop -W catalog.txt /mnt/data/COSMOS/*_drz.fits $ astimgcrop --section=10:*-10,10:*-10 --hdu=2 image.fits $ astimgcrop --ra=189.16704 --dec=62.218203 goodsnorth.fits $ astimgcrop --xc=568.342 --yc=2091.719 --iwidth=200 image.fits @end example @noindent ImageCrop has one mandatory argument which is the input image name(s), shown above with @file{ASTRdata ...}. You can use shell expansions, for example @command{*} for this if you have lots of images in WCS mode. If the crop box centers are in a catalog, you also have to provide the catalog name as an argument. Alternatively, you have to provide the crop box parameters with command-line options. @cindex Asynchronous thread allocation When in catalog mode, ImageCrop will run in parallel unless you set @option{--numthreads=1}, see @ref{Threads in Gnuastro}. Note that when multiple threads are being used, in verbose mode, the outputs will not be in order. This is because the threads are asynchronous and thus not started in order. This has no effect on the output, see @ref{Hubble visually checks and classifies his catalog} for a tutorial on effectively using this feature. @menu * astimgcrop options:: A list of all the options with explanation. * astimgcrop output:: The outputs of ImageCrop. @end menu @node astimgcrop options, astimgcrop output, Invoking astimgcrop, Invoking astimgcrop @subsubsection ImageCrop options The options can be classified into the following contexts: Input, Output and operating mode options. Options that are common to all Gnuastro program are listed in @ref{Common options} and will not be repeated here. @cartouche @noindent @strong{NOTE:} The coordinates are in the FITS format. So the first axis is the horizontal axis when viewed in SAO ds9 and the second axis is the vertical. Also in the FITS standard, counting begins from 1 (one) not 0 (zero). @end cartouche @noindent Input image parameters: @table @option @item --hstartwcs (@option{=INT}) Specify the first keyword card (line number) to start finding the input image world coordinate system information. Distortions were only recently included in WCSLIB (from version 5). Therefore until now, different telescope would apply their own specific set of WCS keywords and put them into the image header along with those that WCSLIB does recognize. So now that WCSLIB recognizes most of the standard distortion parameters, they will get confused with the old ones and give completely wrong results. For example in the CANDELS-GOODS South images@footnote{@url{https://archive.stsci.edu/pub/hlsp/candels/goods-s/gs-tot/v1.0/}}. The two @option{--hstartwcs} and @option{--hendwcs} are thus provided so when using older datasets, you can specify what region in the FITS headers you want to use to read the WCS keywords. Note that this is only relevant for reading the WCS information, basic data information like the image size are read separately. These two options will only be considered when the value to @option{--hendwcs} is larger than that of @option{--hstartwcs}. So if they are equal or @option{--hstartwcs} is larger than @option{--hendwcs}, then all the input keywords will be parsed to get the WCS information of the image. @item --hendwcs (@option{=INT}) Specify the last keyword card to read for specifying the image world coordinate system on the input images. See @option{--hstartwcs} @end table @noindent Crop box parameters: @table @option @item -x @itemx --xc (@option{=FLT}) The first FITS axis value of central position of the crop box in single image mode. @item -y @itemx --yc (@option{=FLT}) The second FITS axis value of the central position of the crop box in single image mode. @item -s @itemx --section (@option{=STR}) Section of the input image which you want to be cropped. See @ref{Crop section syntax} for a complete explanation on the syntax required for this input. @item -l @itemx --polygon (@option{=STR}) String of crop polygon vertices. Note that currently only convex polygons should be used. In the future we will make it work for all kinds of polygons. Convex polygons are polygons that do not have an internal angle more than 180 degrees. This option can be used both in the image and WCS modes. The rectangular region that completely encompasses the polygon will be kept and all the pixels that are outside of it will be removed. The syntax for the polygon vertices is similar to and simpler than that for @option{--section}. In short, the dimensions of each coordinate are separated by a comma (@key{,}) and each vertice is separated by a colon (@key{:}). You can define as many vertices as you like. If you would like to use space characters between the dimensions and vertices to make them more human-readable, then you have to put the value to this option in double quotation marks. For example let's assume you want to work on the deepest part of the WFC3/IR images of Hubble Space Telescope eXtreme Deep Field (HST-XDF). @url{https://archive.stsci.edu/prepds/xdf/, According to the webpage}@footnote{@url{https://archive.stsci.edu/prepds/xdf/}} the deepest part is contained within the coordinates: @example [ (53.187414,-27.779152), (53.159507,-27.759633), (53.134517,-27.787144), (53.161906,-27.807208) ] @end example They have provided mask images with only these pixels in the WFC3/IR images, but what if you also need to work on the same region in the full resolution ACS images? Also what if you want to use the CANDELS data for the shallow region? Running ImageCrop with @option{--polygon} will easily pull out this region of the image for you irrespective of the resolution (if you have set the operating mode to WCS mode in your nearest configuration file, there is no need for @option{--wcsmode}, you may also provide many FITS image or tiles and ImageCrop will stitch them all): @example $ astimgcrop --wcsmode desired-filter-image(s).fits \ --polygon="53.187414,-27.779152 : 53.159507,-27.759633 : \ 53.134517,-27.787144 : 53.161906,-27.807208" @end example @item --outpolygon Keep all the regions outside the polygon and mask the inner ones with blank pixels (see @ref{Blank pixels}). This is practically the inverse of the default mode of treating polygons. Note that this option only works when you have only provided one input image. If multiple images are given (in WCS mode), then the full area covered by all the images has to be shown and the polygon excluded. This can lead to a very large area if large surveys like COSMOS are used. So ImageCrop will abort and notify you. In such cases, it is best to crop out the larger region you want, then mask the smaller region with this option. @item -r @itemx --ra (@option{=FLT}) The first FITS axis value of central position of the crop box in single image mode. @item -d @itemx --dec (@option{=FLT}) The second FITS axis value of the central position of the crop box in single image mode. @item -i @itemx --xcol (@option{=INT}) Column number of the first FITS axis position of the box center, starting from zero. In SAO ds9, the first FITS axis is the horizontal axis. @item -j @itemx --ycol (@option{=INT}) Column number of the second FITS axis position of the box center, starting from zero. In SAO ds9, the second FITS axis is the vertical axis. @item -a @itemx --iwidth (@option{=INT}) Width the square box to crop in image mode in units of pixels. In order for the chosen central pixel to be in the center of the cropped image, the final width has to be an odd number, therefore if the value to this option is an even number, the final crop width will be one pixel larger in each dimension. If you want an even sided crop box, use the @option{--section} option to specify the boundaries of the box, see @ref{Crop section syntax}. @item -f @itemx --racol (@option{=INT}) Column number of Right Ascension (RA) in the input catalog, starting from zero. @item -g @itemx --deccol (@option{=INT}) Column number of declination in the input catalog, starting from zero. @item -w @itemx --wwidth (@option{=FLT}) The width of the crop box in WCS mode in units of arc-seconds. @end table @noindent Output options: @table @option @item -c @itemx --checkcenter @cindex Check center of crop (@option{=INT}) Box size of region in the center of the image to check in units of pixels. This is only used in WCS mode. Because surveys don't often have a clean square or rectangle shape, some of the pixels on the sides of the surveys don't have any data and are commonly filled with zero valued pixels. If the RA and Dec of any of the targets specified in the catalog fall in such regions, that cropped image will be useless! Therefore with this option, you can specify a width of a small box (3 pixels is often good enough) around the central pixel of the cropped image. If all the pixels in this small box have the value of zero, no cropped image will be created and this object will be flagged in the final log file. @item -p @itemx --suffix (@option{=STR}) The suffix (or post-fix) of the output files for when you want all the cropped images to have a special ending. One case where this might be helpful is when besides the science images, you want the weight images (or exposure maps, which are also distributed with survey images) of the cropped regions too. So in one run, you can set the input images to the science images and @option{--suffix=_s.fits}. In the next run you can set the weight images as input and @option{--suffix=_w.fits}. @item -b @itemx --noblank Pixels outside of the input image that are in the crop box will not be used. By default they are filled with blank values (depending on type), see @ref{Blank pixels}. @item -z @itemx --zeroisnotblank In float or double images, it is common to give the value of zero to blank pixels. If the input image type is one of these two types, such pixels will also be considered as blank. You can disable this behavior with this option, see @ref{Blank pixels}. @end table @noindent Operating mode options: @table @option @item -I @itemx --imgmode Operate in Image mode as described above. This option is only useful when catalog is being provided. If coordinates are given on the command-line, the mode is automatically set based on them. @item -W @itemx --wcsmode Operate in WCS mode. See explanations for @option{--imgmode}. @end table @node astimgcrop output, , astimgcrop options, Invoking astimgcrop @subsubsection ImageCrop output When a catalog is given, the value of @option{--output} (see @ref{Common options}) will be seen as the directory to store the output cropped images. In such cases, the outputs will consist of two parts: a variable part (the row number of each target starting from 1) along with a fixed string which you can set with the @option{--suffix} option. Note that in catalog mode, only one image can be input. When the crop box is specified on the command-line, the value to @option{--output} will be used as a file name. If no output is specified or if it is a directory, the output file name will follow the automatic output names of Gnuastro, see @ref{Automatic output} for the input image. The header of each output cropped image will contain the names of the input image(s) it was cut from. If a name is longer than the 70 character space that the FITS standard allows for header keyword values, the name will be cut into several keywords from the nearest slash (@key{/}). The keywords have the following format: @command{ICFn_m}. Where @command{n} is the number of the image used in this crop and @command{m} is the part of the name. Following the name is another keyword named @command{ICFnPIX} which shows the pixel range from that input image in the same syntax as @ref{Crop section syntax}. Once done, a log file will be created in the current directory named @file{astimgcrop.log}. For each input row, this file will have three columns: @enumerate @item The cropped image file name for that row. @item The number of input images that were used to create that image. @item A @code{0} if the central few pixels (value to the @option{--checkcenter} option) are blank and @code{1} otherwise. @end enumerate There are also comments on the top explaining basic information about the run. If the log file cannot be created (for example you don't have write permission in the directory you are running ImageCrop in) or you have specifically asked for no log file (with the @option{--nolog} option), then a log file will not be created (unless @option{--individual} is called). The same columns will be printed in verbose mode on the command-line for each row. @node Arithmetic, Convolve, ImageCrop, Image manipulation @section Arithmetic It is commonly necessary to do arithmetic operations on the astronomical data. For example in the reduction of raw data it is necessary to subtract the Sky value (@ref{Sky value}) from each image image. Later (once the images as warped into a single grid using ImageWarp for example, see @ref{ImageWarp}), the images can be co-added or the output pixel grid is the average of the pixels of the individual input images. Arithmetic currently uses the reverse polish or postfix notation, see @ref{Reverse polish notation}, for more information on how to run Arithmetic, please see @ref{Invoking astarithmetic}. @menu * Reverse polish notation:: The current notation style for Arithmetic * Arithmetic operators:: List of operators known to Arithmetic * Invoking astarithmetic:: How to run Arithmetic: options and output @end menu @node Reverse polish notation, Arithmetic operators, Arithmetic, Arithmetic @subsection Reverse polish notation @cindex Postfix notation @cindex Reverse Polish Notation The most common notation for arithmetic operations is the infix notation@footnote{@url{https://en.wikipedia.org/wiki/Infix_notation}} where the operator goes between the two operands, for example @mymath{4+5}. While the infix notation is the preferred way in most programming languages, currently Arithmetic does not use it since it will require parenthesis which can complicate the implementation of the code. In the near future we do plan to adopt this notation@footnote{@url{https://savannah.gnu.org/task/index.php?13867}}, but for the time being (due to time constraints on the developers), Arithmetic uses the postfix or reverse polish notation@footnote{@url{https://en.wikipedia.org/wiki/Reverse_Polish_notation}}. The referenced Wikipedia article provides some excellent explanation on this notation but here we will give a short summary for self-sufficiency. In the postfix notation, the operator is placed after the operands, as we will see below this removes the need to define parenthesis for most ordinary operators. For example, instead of writing @command{5+6}, we write @command{5 6 +}. To easily understand how this notation works, you can think of each operand as a node in a first-in-first-out stack. Every time an operator is confronted, it pops the number of operands it needs from the top of the stack (so they don't exist in the stack any more), does its operation and pushes the result back on top of the stack. So if you want the average of 5 and 6, you would write: @command{5 6 + 2 /}. The operations that are done are: @enumerate @item @command{5} is an operand, so it is pushed to the top of the stack. @item @command{6} is an operand, so it is pushed to the top of the stack. @item @command{+} is a binary operator, so pull the top two elements of the stack and perform addition on them (the order is @command{5+6} in the example above). The result is @command{11}, push it on top of the stack. @item @command{2} is an operand so push it onto the top of the stack. @item @command{/} is a binary operator, so pull out the top two elements of the stack (top-most is @command{2}, then @command{11}) and divide the second one by the first. @end enumerate In Gnuastro's Arithmetic, the operands can be FITS images or numbers. As you can see, very complicated procedures can be created without the need for parenthesis. Even functions which take an arbitrary number of arguments can be defined in this notation. For example the Postscript language@footnote{See the EPS and PDF part of @ref{Recognized file types} for a little more on the Postscript language.} (the programming language in Postscript and compiled into PDF files) uses this notation. @node Arithmetic operators, Invoking astarithmetic, Reverse polish notation, Arithmetic @subsection Arithmetic operators The recognized operators in Arithmetic are listed below. See @ref{Reverse polish notation} for more on how the operators and operands should be ordered on the command-line. The operands to all operators can be a data array (for example a FITS image) or a number, the output will be an array or number according to the inputs. For example a number multiplied by an array will produce an array. The conditional operators will return pixel, or numerical values of 0 (false) or 1 (true). @table @command @item + Addition, so ``@command{4 5 +}'' is equivalent to @mymath{4+5}. @item - Subtraction, so ``@command{4 5 -}'' is equivalent to @mymath{4-5}. @item * Multiplication, so ``@command{4 5 "*"}'' is equivalent to @mymath{4\times5}. On the command-line or in scripts, be sure to quote the multiplication sign (for example @command{"*"}). @item / Division, so ``@command{4 5 /}'' is equivalent to @mymath{4/5}. @item abs Absolute value of first operand, so ``@command{4 abs}'' is equivalent to @mymath{|4|}. @item pow First operand to the power of the second, so ``@command{4 5 pow}'' is equivalent to @mymath{4^5}. @item sqrt The square root of the first operand, so ``@command{4 sqrt}'' is equivalent to @mymath{\sqrt{4}}. @item log Natural logarithm of first operand, so ``@command{4 log}'' is equivalent to @mymath{\ln(4)}. @item log10 Base-10 logarithm of first operand, so ``@command{4 log10}'' is equivalent to @mymath{\log(4)}. @item minvalue Minimum value in the top operand on the stack, so ``@command{a.fits min}'' will push the the minimum pixel value in this image onto the stack. Therefore this operator is mainly intended for data (for example images), if the top operand is a number, this operator just returns it without any change. So note that when this operator acts on a single image, the output will no longer be an image, but a number. @item maxvalue Maximum value of first operand, similar to @command{minvalue}. @cindex NaN @item min If there are several operands (images), each pixel of the output of this operator will be set to the minimum value of all the operands (images) in that pixel. If the operands are all numbers, then their minimum value will be put in the stack. So ``@command{a.fits b.fits c.fits min}'' will produce an image with the same size as the inputs but each output pixel is set to the minimum respective pixel value of the three input images. Important notes: @itemize @item All the operands must be either images or numbers, they cannot be mixed. @item NaN/blank pixels will be ignored, see @ref{Blank pixels}. @item All available operands on the stack will be pulled for this operator to generate its output. So after calling this operator, there will only be one operand on the stack, see @ref{Reverse polish notation}. @end itemize @item max Similar to @command{min}, but the pixels of the output will contain the maximum of the respective pixels in all operands in the stack. @item average Similar to @command{min}, but the pixels of the output will contain the average of the respective pixels in all operands in the stack. @item median Similar to @command{min}, but the pixels of the output will contain the median of the respective pixels in all operands in the stack. @item lt Less than: If the second popped (or left operand in infix notation, see @ref{Reverse polish notation}) value is smaller than the first popped operand, then this function will return a value of 1, otherwise it will return a value of 0. If both operands are images, then all the pixels will be compared with their counterparts in the other image. If only one operand is an image, then all the pixels will be compared with the the single value (number) of the other operand. Finally if both are numbers, then the output is also just one number (0 or 1). @item le Less or equal: similar to @code{lt} (`less than' operator), but returning 1 when the second popped operand is smaller or equal to the first. @item gt Greater than: similar to @code{lt} (`less than' operator), but returning 1 when the second popped operand is greater than the first. @item ge Greater or equal: similar to @code{lt} (`less than' operator), but returning 1 when the second popped operand is larger or equal to the first. @item eq Equality: similar to @code{lt} (`less than' operator), but returning 1 when the two popped operands are equal (to double precision floating point accuracy). @item neq Non-Equality: similar to @code{lt} (`less than' operator), but returning 1 when the two popped operands are @emph{not} equal (to double precision floating point accuracy). @cindex Blank pixel @item isblank Test for a blank value (see @ref{Blank pixels}). In essence, this is very similar to the conditional operators: the output is either 1 or 0 (see the `less than' operator above). The difference is that it only needs one operand. Because of the definition of a blank pixel, a blank value is not even equal to itself, so you cannot use the equal operator above to select blank pixels. See the ``Blank pixels'' box below for more on Blank pixels in Arithmetic. @item and Logical AND: returns 1 if both operands have a non-zero value and 0 if both are zero. Both operands have to be the same kind: either both images or both numbers. @item or Logical OR: returns 1 if either one of the operands is non-zero and 0 only when both operators are zero. Both operands have to be the same kind: either both images or both numbers. @item not Logical NOT: returns 1 when the operand is zero and 0 when the operand is non-zero. The operand can be an image or number, for an image, it is applied to each pixel separately. @item where Change the input (pixel) value `where' a certain condition holds. The conditional operators above can be used to define the condition. Three operands are required for @command{where}. The input format is demonstrated in this simplified example: @example $ astarithmetic in.fits condition.fits new.fits where @end example The third and second popped operands (@file{in.fits} and @file{condition.fits} above, see @ref{Reverse polish notation}) have to be images or all three operands have to be numbers. In the former case (when the first two are images), the third operand can be an image or a number. The value of any pixel in @file{in.fits} that corresponds to a non-zero pixel of @file{condition.fits} will be changed to the value of the same pixel in @file{new.fits} (or a fixed number if the first popped operand is a number). Commonly you won't be dealing with an actual FITS file of a conditional image. You will probably define the condition in the same run based on some other reference image and use the conditional and logical operators above to make a true/false (or one/zero) image for you internally. For example the case below: @example $ astarithmetic in.fits reference.fits 100 gt new.fits where @end example @end table @cartouche @noindent @strong{Important reminder for multiplication:} please quote the @command{*} sign (for example, @command{"*"} or @command{'*'}). Without quotation, the shell will replace @command{*} with a list of all the files in your working directory which can produce unpredictable outputs. In any case, the input images are not affected, they are only read. @end cartouche @cartouche @noindent @strong{Blank pixels in Arithmetic:} Currently all Arithmetic operations are internally done in double precision floating points. So all blank pixels in the image (see @ref{Blank pixels}) will be stored as IEEE NaN values. One particular aspect of NaN values is that by definition they will fail on @emph{any} comparison. Hence both equal and not-equal operators will fail when both their operands are NaN! The only way to select blank pixels is through the @command{isblank} operator explained above. One way you can exploit this property of the NaN value to your advantage is when you want a fully zero-valued image (even over the blank pixels) based on an already existing image (with same size and world coordinate system settings). The following command will produce this for you: @example $ astarithmetic input.fits nan eq --output=all-zeros.fits @end example @noindent Note that on the command-line you can write NaN in any case (for example @command{NaN}, or @command{NAN} are also acceptable). Reading NaN as a floating point number in Gnuastro isn't case-sensitive. @end cartouche @node Invoking astarithmetic, , Arithmetic operators, Arithmetic @subsection Invoking Arithmetic Arithmetic will do pixel to pixel arithmetic operations on the individual pixels of input data and/or numbers. All input data files must have the same dimensions. The general template is: @example $ astarithmetic [OPTION...] ASTRdata1 [ASTRdata2] OPERATOR ... @end example @noindent One line examples: @example $ astarithmetic 10.32 3.84 - 2.7 pow # will print 155.329 $ astarithmetic 1 image.fits / --out=inverse.fits $ astarithmetic image.fits -1 "*" --out=negative.fits $ astarithmetic image.fits image.fits - --out=skysub.fits \ --hdu=0 --hdu=3 $ astarithmetic image1.fits image2.fits + 2 / --out=average.fits $ astarithmetic image1.fits image2.fits average --out=average.fits $ astarithmetic img1.fits img2.fits img3.fits median \ -h0 -h1 -h2 --out=median.fits @end example If the output is an image, and the @option{--output} option is not given, automatic output will use the name of the first FITS image encountered to generate an output file name, see @ref{Automatic output}. Also, output WCS information will be taken from the first input image encountered. If the output is a single number, that number will be printed in the standard output. See @ref{Reverse polish notation} for the notation used to mix operands and operators on the command-line. @cindex NaN @cindex Mask image Currently Arithmetic will convert the input image into double precision floating point arrays for the operations. But there are plans to allow it to also operate on integer (labeled or masked) images with bit-wise operators so mask layers can also be manipulated@footnote{@url{https://savannah.gnu.org/task/?13869}}. Unless otherwise stated for each operator, blank pixels in the input image will automatically be set as blank in the output. To ignore certain pixels (see @ref{Blank pixels}), you can specify a mask image, see @ref{Mask image}. In that case, when reading the first FITS image, all the masked pixels will be changed to a NaN value. Therefore in any further operations with other images, the output for those pixels will always be a NaN (blank pixel value for floating point data type). Currently all the operations in Arithmetic are done in double precision floating point type. However, if none of the input images have this type, the output will be stored as a single precision floating point type. @cindex Options The hyphen (@command{-}) can be used both to specify options (see @ref{Options}) and also to specify a negative number which might be necessary in your arithmetic. In order to enable you to do this, Arithmetic will first parse all the input strings and if the first character after a hyphen is a digit, then that hyphen is temporarily replaced by the vertical tab character which is not commonly used. The arguments are then parsed and these strings will not be specified as an option. Then the given arguments are parsed and any vertical tabs are replaced back with a hyphen so they can be read as negative numbers. So as long as the names of the files you want to work on do not start with a vertical tab followed by a digit, there is no problem. An important consequence of this implementation is that you should not write negative fractions like this: @command{-.3}, instead write them as @command{-0.3}. @cindex AWK @cindex GNU AWK Without any images, Arithmetic will act like a simple calculator and print the resulting output number on the standard output like the first example above. If you really want such calculator operations on the command-line, AWK (GNU AWK is the most common implementation) is much faster, easier and much more powerful. For example, the numerical one-line example above can be done with the following command. In general AWK is a fantastic tool and GNU AWK has a wonderful manual (@url{https://www.gnu.org/software/gawk/manual/}). So if you confront situations like this a lot or have to work with large text tables/catalogs, be sure to checkout AWK and simplify your life. @example $ echo "" | awk '@{print (10.32-3.84)^2.7@}' 155.329 @end example See @ref{Common options} for a review of the options in all Gnuastro programs, the two options related to a mask image are also specified in @ref{Mask image}. Arithmetic just redefines the @option{--hdu} option as explained below: @table @option @item -h @itemx --hdu (@option{=INT}) Unlike most options in Gnuastro (which will ultimately only have one value for this option), Arithmetic allows @option{--hdu} to be called multiple times and the value of each invocation will be stored separately (for the unlimited number of input images you would like to use). The order of the values to @option{--hdu} is very important (if they don't have the same value!). The order is determined by the order that this option is read: first on the command-line (from left to right), then top-down in each configuration file, see @ref{Configuration file precedence}. If the number of HDUs is less than the number of input images, Arithmetic will abort and notify you. However, if there are more HDUs than FITS images, there is no problem: they will be used in the given order (every time a FITS image comes up on the stack) and the extra HDUs will be ignored in the end. So there is no problem with having extra HDUs in the configuration files and by default several HDUs with a value of @option{0} are kept in the system-wide configuration file when you install Gnuastro. @end table @node Convolve, ImageWarp, Arithmetic, Image manipulation @section Convolve @cindex Convolution @cindex Neighborhood @cindex Weighted average @cindex Average, weighted @cindex Kernel, convolution On an image, convolution can be thought of as a process to blur or remove the contrast in an image. If you are already familiar with the concept and just want to run Convolve, you can jump to @ref{Convolution kernel} and @ref{Invoking astconvolve} and skip the lengthy introduction on the basic definitions and concepts of convolution. There are generally two methods to convolve an image. The first and more intuitive one is in the ``spatial domain'' or using the actual image pixel values, see @ref{Spatial domain convolution}. The second method is when we manipulate the ``frequency domain'', or work on the magnitudes of the different frequencies that constitute the image, see @ref{Frequency domain and Fourier operations}. Understanding convolution in the spatial domain is more intuitive and thus recommended if you are just starting to learn about convolution. However, getting a good grasp of the frequency domain is a little more involved and needs some concentration and some mathematical proofs. However, its reward is a faster operation and more importantly a very fundamental understanding of this very important operation. @cindex Detection @cindex Atmosphere @cindex Blur image @cindex Cosmic rays @cindex Pixel mixing @cindex Mixing pixel values Convolution of an image will generally result in blurring the image because it mixes pixel values. In other words, if the image has sharp differences in neighboring pixel values@footnote{In astronomy, the only major time we confront such sharp borders in signal are cosmic rays. All other sources of signal in an image are already blurred by the atmosphere or the optics of the instrument.}, those sharp differences will become smoother. This has very good consequences in detection of signal in noise for example. In an actual observed image, the variation in neighboring pixel values due to noise can be very high. But after convolution, those variations will decrease and we have a better hope in detecting the possible underlying signal. Another case where convolution is extensively used is in mock images and modeling in general, convolution can be used to simulate the effect of the atmosphere or the optical system on the mock profiles that we create, see @ref{PSF}. Convolution is a very interesting and important topic in any form of signal analysis (including astronomical observations). So we have thoroughly@footnote{A mathematical will certainly consider this explanation is incomplete and inaccurate. However this text is written for an understanding on the operations that are done on a real (not complex, discrete and noisy) astronomical image, not any general form of abstract function} explained the concepts behind it in the following sub-sections. @menu * Spatial domain convolution:: Only using the input image values. * Frequency domain and Fourier operations:: Using frequencies in input. * Spatial vs. Frequency domain:: When to use which? * Convolution kernel:: How to specify the convolution kernel. * Invoking astconvolve:: Options and argument to Convolve. @end menu @node Spatial domain convolution, Frequency domain and Fourier operations, Convolve, Convolve @subsection Spatial domain convolution The pixels in an input image represent different ``spatial'' positions, therefore when convolution is done only using the actual input pixel values, we name the process as being done in the ``Spatial domain''. In particular this is in contrast to the ``frequency domain'' that we will discuss later in @ref{Frequency domain and Fourier operations}. In the spatial domain (and in realistic situations where the image and the convolution kernel don't extend to infinity), convolution is the process of changing the value of one pixel to the @emph{weighted} average of all the pixels in its @emph{neighborhood}. The `neighborhood' of each pixel (how many pixels in which direction) and the `weight' function (how much each neighboring pixel should contribute depending on its position) are given through a second image which is known as a ``kernel''@footnote{Also known as filter, here we will use `kernel'.}. @menu * Convolution process:: More basic explanations. * Edges in the spatial domain:: Dealing with the edges of an image. @end menu @node Convolution process, Edges in the spatial domain, Spatial domain convolution, Spatial domain convolution @subsubsection Convolution process In convolution, the kernel specifies the weight and positions of the neighbors of each pixel. To find the convolved value of a pixel, the central pixel of the kernel is placed on that pixel. The values of each overlapping pixel in the kernel and image are multiplied by each other and summed for all the kernel pixels. To have one pixel in the center, the sides of the convolution kernel have to be an odd number. This process effectively mixes the pixel values of each pixel with its neighbors, resulting in a blurred image compared to the sharper input image. @cindex Linear spatial filtering Formally, convolution is one kind of linear `spatial filtering' in image processing texts. If we assume that the kernel has @mymath{2a+1} and @mymath{2b+1} pixels on each side, the convolved value of a pixel placed at @mymath{x} and @mymath{y} (@mymath{C_{x,y}}) can be calculated from the neighboring pixel values in the input image (@mymath{I}) and the kernel (@mymath{K}) from @dispmath{C_{x,y}=\sum_{s=-a}^{a}\sum_{t=-b}^{b}K_{s,t}\times{}I_{x+s,y+t}.} @cindex Correlation @cindex Convolution Any pixel coordinate that is outside of the image in the equation above will be considered to be zero. When the kernel is symmetric about its center the blurred image has the same orientation as the original image. However, if the kernel is not symmetric, the image will be affected in the opposite manner, this is a natural consequence of the definition of spatial filtering. In order to avoid this we can rotate the kernel about its center by 180 degrees so the convolved output can have the same original orientation. Technically speaking, only if the kernel is flipped the process is known @emph{Convolution}. If it isn't it is known as @emph{Correlation}. To be a weighted average, the sum of the weights (the pixels in the kernel) have to be unity. This will have the consequence that the convolved image of an object and un-convolved object will have the same brightness (see @ref{Flux Brightness and magnitude}), which is natural, because convolution should not eat up the object photons, it only disperses them. @node Edges in the spatial domain, , Convolution process, Spatial domain convolution @subsubsection Edges in the spatial domain In purely `linear' spatial filtering (convolution), there are problems on the edges of the input image. Here we will explain the problem in the spatial domain, see @ref{Edges in the frequency domain}. The problem originates from the fact that on the edges, in practice@footnote{Because we assumed the overlapping pixels outside the input image have a value of zero.}, the sum of the weights we use on the actual image pixels is not unity. For example, as discussed above, a profile in the center of an image will have the same brightness before and after convolution. However, for a profile on the edge of the image, the brightness (sum of its pixel fluxes within the image, see @ref{Flux Brightness and magnitude}) will not be equal, some of the flux is going to be `eaten' by the edges. If you ran @command{$ make check} on the source files of Gnuastro, you can see the this effect by comparing the @file{convolve_frequency.fits} with @file{convolve_spatial.fits} in the @file{./tests/} directory. In the spatial domain, by default, no assumption will be made about pixels outside of the image or any blank pixels in the image, see @ref{Blank pixels}. The problem explained above will also occur on the sides of blank regions (which might be masked for example). The solution to this edge effect problem is only possible in the spatial domain. We have to discard the assumption that the sum of the kernel pixels is unity during the convolution process@footnote{ofcourse the sum of the kernel pixels still have to be unity.}. So taking @mymath{W} as the sum of the kernel pixels that used non-blank and in-image pixels, the equation in @ref{Convolution process} will become: @dispmath{C_{x,y}= { \sum_{s=-a}^{a}\sum_{t=-b}^{b}K_{s,t}\times{}I_{x+s,y+t} \over W}.} @noindent In this manner, objects which are near the sides of the image or blank pixels will also have the same brightness (within the image) before and after convolution. This correction is applied by default in Convolve when convolving in the spatial domain. To disable it, you can use the @option{--noedgecorrection} option. In the frequency domain, there is no way to avoid this loss of flux near the edges of the image, see @ref{Edges in the frequency domain}. Note that the edge effect discussed here is different from the one in @ref{If convolving afterwards}. In making mock images we want to simulate a real observation. In a real observation the images of the galaxies on the sides of the CCD are first blurred by the atmosphere and instrument, then imaged. So light from the parts of a galaxy which are immediately outside the CCD will affect the parts of the galaxy which are covered by the CCD. Therefore in modeling the observation, we have to convolve an image that is larger than the input image by exactly half of the convolution kernel. We can hence conclude that this correction for the edges is only useful when working on actual observed images (where we don't have any more data on the edges) and not in modeling. @node Frequency domain and Fourier operations, Spatial vs. Frequency domain, Spatial domain convolution, Convolve @subsection Frequency domain and Fourier operations Getting a good grip on the frequency domain is usually not an easy job! So we have decided to give the issue a complete review here. Convolution in the frequency domain (see @ref{Convolution theorem}) heavily relies on the concepts of Fourier transform (@ref{Fourier transform}) and Fourier series (@ref{Fourier series}) so we will be investigating these important operations first. It has become something of a clich@'e for people to say that the Fourier series ``is a way to represent a (wave-like) function as the sum of simple sine waves'' (from Wikipedia). However, sines themselves are abstract functions, so this statement really adds no extra layer of physical insight. Before jumping head-first into the equations and proofs, we will begin with a historical background to see how the importance of frequencies actually roots in our ancient desire to see everything in terms of circles. A short review of how the complex plane should be interpreted is then given. Having paved the way with these two basics, we define the Fourier series and subsequently the Fourier transform. The final aim is to explain discrete Fourier transform, however some very important concepts need to be solidified first: The Dirac comb, convolution theorem and sampling theorem. So each of these topics are explained in their own separate sub-sub-section before going on to the discrete Fourier transform. Finally we revisit (after @ref{Edges in the spatial domain}) the problem of convolution on the edges, but this time in the frequency domain. Understanding the sampling theorem and the discrete Fourier transform is very important in order to be able to pull out valuable science from the discrete image pixels. Therefore we have included the mathematical proofs and figures so you can have a clear understanding of these very important concepts. @menu * Fourier series historical background:: Historical background. * Circles and the complex plane:: Interpreting complex numbers. * Fourier series:: Fourier Series definition. * Fourier transform:: Fourier Transform definition. * Dirac delta and comb:: Dirac delta and Dirac comb. * Convolution theorem:: Derivation of Convolution theorem. * Sampling theorem:: Sampling theorem (Nyquist frequency). * Discrete Fourier transform:: Derivation and explanation of DFT. * Fourier operations in two dimensions:: Extend to 2D images. * Edges in the frequency domain:: Interpretation of edge effects. @end menu @node Fourier series historical background, Circles and the complex plane, Frequency domain and Fourier operations, Frequency domain and Fourier operations @subsubsection Fourier series historical background Ever since the ancient times, the circle has been (and still is) the simplest shape for abstract comprehension. All you need is a center point and a radius and you are done. All the points on a circle are at a fixed distance from the center. However, the moment you try to connect this elegantly simple and beautiful abstract construct (the circle) with the real world (for example compute its area or its circumference), things become really hard (ideally, impossible) because the irrational number @mymath{\pi} gets involved. The key to understanding the Fourier series (thus the Fourier transform and finally the Discrete Fourier Transform) is our ancient desire to express everything in terms of circles or the most exceptionally simple and elegant abstract human construct. Most people prefer to say the same thing in a more ahistorical manner: to break a function into sines and cosines. As the term ``ancient'' in the previous sentence implies, Jean-Baptiste Joseph Fourier (1768 -- 1830 A.D.) was not the first person to do this. The main reason we know this process by his name today is that he came up with an ingenious method to find the necessary coefficients (radius of) and frequencies (``speed'' of rotation on) the circles for any generic (integrable) function. @float Figure,epicycle @c Since these links are long, we had to write them like this so they don't @c jump out of the text width. @image{gnuastro-figures/epicycles, 15.2cm, , Middle ages epicycles along with two demonstrations of breaking a generic function using epicycles.} @caption{Epicycles and the Fourier series. Left: A demonstration of Mercury's epicycles relative to the ``center of the world'' by Qutb al-Din al-Shirazi (1236 -- 1311 A.D.) retrieved @url{https://commons.wikimedia.org/wiki/File:Ghotb2.jpg, from Wikipedia}. @url{https://commons.wikimedia.org/wiki/File:Fourier_series_square_wave_circles_animation.gif, Middle} and Right: How adding more epicycles (or terms in the Fourier series) will approximate functions. The @url{https://commons.wikimedia.org/wiki/File:Fourier_series_sawtooth_wave_circles_animation.gif, right} animation is also available.} @end float Like most aspects of mathematics, this process of interpreting everything in terms of circles, began for astronomical purposes. When astronomers noticed that the orbit of Mars and other outer planets, did not appear to be a simple circle (as everything should have been in the heavens). At some point during their orbit, the revolution of these planets would become slower, stop, go back a little (in what is known as the retrograde motion) and then continue going forward again. The correction proposed by Ptolemy (90 -- 168 A.D.) was the most agreed upon. He put the planets on Epicycles or circles whose center itself rotates on a circle whose center is the earth. Eventually, as observations became more and more precise, it was necessary to add more and more epicycles in order to explain the complex motions of the planets@footnote{See the Wikipedia page on ``Deferent and epicycle'' for a more complete historical review.}. @ref{epicycle}(Left) shows an example depiction of the epicycles of Mercury in the late 13th century. Of course we now know that if they had abdicated the Earth from its throne in the center of the heavens and allowed the Sun to take its place, everything would become much simpler and true. But there wasn't enough observational evidence for changing the ``professional consensus'' of the time to this radical view suggested by a small minority@footnote{Aristarchus of Samos (310 -- 230 B.C.) appears to be one of the first people to suggest the Sun being in the center of the universe. This approach to science (that the standard model is defined by consensus) and the fact that this consensus might be completely wrong still applies equally well to our models of particle physics and cosmology today.}. So the pre-Galilean astronomers chose to keep Earth in the center and find a correction to the models (while keeping the heavens a purely ``circular'' order). The main reason we are giving this historical background which might appear off topic is to give historical evidence that while such ``approximations'' do work and are very useful for pragmatic reasons (like measuring the calendar from the movement of astronomical bodies). They offer no physical insight. The astronomers who were involved with the Ptolemaic world view had to add a huge number of epicycles during the centuries after Ptolemy in order to explain more accurate observations. Finally the death knell of this world-view was Galileo's observations with his new instrument (the telescope). So the physical insight, which is what Astronomers and Physicists are interested in (as opposed to Mathematicians and Engineers who just like proving and optimizing or calculating!) comes from being creative and not limiting our selves to such approximations. Even when they work. @node Circles and the complex plane, Fourier series, Fourier series historical background, Frequency domain and Fourier operations @subsubsection Circles and the complex plane Before going onto the derivation, it is also useful to review how the complex numbers and their plane relate to the circles we talked about above. The two schematics in the middle and right of @ref{epicycle} show how a 1D function of time can be made using the 2D real and imaginary surface. Seeing the animation in Wikipedia will really help in understanding this important concept. At each point in time, we take the vertical coordinate of the point and use it to find the value of the function at that point in time. @ref{iandtime} shows this relation with the axes marked. Leonhard Euler@footnote{Other forms of this equation were known before Euler. For example in 1707 A.D. (the year of Euler's birth) Abraham de Moivre (1667 -- 1754 A.D.) showed that @mymath{(\cos{x}+i\sin{x})^n=\cos(nx)+i\sin(nx)}. In 1714 A.D., Roger Cotes (1682 -- 1716 A.D. a colleague of Newton who proofread the second edition of Principia) showed that: @mymath{ix=\ln(\cos{x}+i\sin{x})}.} (1707 -- 1783 A.D.) showed that the complex exponential (@mymath{e^{iv}} where @mymath{v} is real) is periodic and can be written as: @mymath{e^{iv}=\cos{v}+isin{v}}. Therefore @mymath{e^{iv+2\pi}=e^{iv}}. Later, Caspar Wessel (mathematician and cartographer 1745 -- 1818 A.D.) showed how complex numbers can be displayed as vectors on a plane. Euler's identity might seem counter intuitive at first, so we will try to explain it geometrically (for a more physical insight). On the real-imaginary 2D plane (like the left hand plot in each box of @ref{iandtime}), multiplying a number by @mymath{i} can be interpretted as rotating the point by @mymath{90} degrees (for example the value @mymath{3} on the real axis becomes @mymath{3i} on the imaginary axis). On the other hand, @mymath{e\equiv\lim_{n\rightarrow\infty}(1+{1\over n})^n}, therefore, defining @mymath{m\equiv nu}, we get: @dispmath{e^{u}=\lim_{n\rightarrow\infty}\left(1+{1\over n}\right)^{nu} =\lim_{n\rightarrow\infty}\left(1+{u\over nu}\right)^{nu} =\lim_{m\rightarrow\infty}\left(1+{u\over m}\right)^{m}} @noindent Taking @mymath{u\equiv iv} the result can be written as a generic complex number (a function of @mymath{v}): @dispmath{e^{iv}=\lim_{m\rightarrow\infty}\left(1+i{v\over m}\right)^{m}=a(v)+ib(v)} @noindent For @mymath{v=\pi}, a nice geometric animation of going to the limit can be seen @url{https://commons.wikimedia.org/wiki/File:ExpIPi.gif, on Wikipedia}. We see that @mymath{\lim_{m\rightarrow\infty}a(\pi)=-1}, while @mymath{\lim_{m\rightarrow\infty}b(\pi)=0}, which gives the famous @mymath{e^{i\pi}=-1} equation. The final value is the real number @mymath{-1}, however the distance of the polygon points traversed as @mymath{m\rightarrow\infty} is half the circumference of a circle or @mymath{\pi}, showing how @mymath{v} in the equation above can be interpretted as an angle in units of radians and therefore how @mymath{a(v)=cos(v)} and @mymath{b(v)=sin(v)}. Since @mymath{e^{iv}} is periodic (let's assume with a period of @mymath{T}), it is more clear to write it as @mymath{v\equiv{2{\pi}n\over T}t} (where @mymath{n} is an integer), so @mymath{e^{iv}=e^{i{2{\pi}n\over T}t}}. The advantage of this notation is that the period (@mymath{T}) is clearly visible and the frequency (@mymath{2{\pi}n \over T}, in units of 1/cycle) is defined through the integer @mymath{n}. In this notation, @mymath{t} is in units of ``cycle''s. As we see from the examples in @ref{epicycle} and @ref{iandtime}, for each constituting frequency, we need a respective `magnitude' or the radius of the circle in order to accurately approximate the desired 1D function. The concepts of ``period'' and ``frequency'' are relatively easy to grasp when using temporal units like time because this is how we define them in every-day life. However, in an image (astronomical data), we are dealing with spatial units like distance. Therefore, by one ``period'' we mean the @emph{distance} at which the signal is identical and frequency is defined as the inverse of that spatial ``period''. The complex circle of @ref{iandtime} can be thought of the Moon rotating about Earth which is rotating around the Sun; so the ``Real (signal)'' axis shows the Moon's position as seen by a distant observer on the Sun as time goes by. Because of the scalar (not having any direction or vector) nature of time, @ref{iandtime} is easier to understand in units of time. When thinking about spatial units, mentally replace the ``Time (sec)'' axis with ``Distance (meters)''. Because length has direction and is a vector, visualizing the rotation of the imaginary circle and the advance along the ``Distance (meters)'' axis is not as simple as temporal units like time. @float Figure,iandtime @image{gnuastro-figures/iandtime, 15.2cm, , } @caption{Relation between the real (signal), imaginary (@mymath{i\equiv\sqrt{-1}}) and time axes at two snapshots of time.} @end float @node Fourier series, Fourier transform, Circles and the complex plane, Frequency domain and Fourier operations @subsubsection Fourier series In astronomical images, our variable (brightness, or number of photo-electrons, or signal to be more generic) is recorded over the 2D spatial surface of a camera pixel. However to make things easier to understand, here we will assume that the signal is recorded in 1D (assume one row of the 2D image pixels). Also for this section and the next (@ref{Fourier transform}) we will be talking about the signal before it is digitized or pixelated. Let's assume that we have the continuous function @mymath{f(l)} which is integrable in the interval @mymath{[l_0, l_0+L]} (always true in practical cases like images). Take @mymath{l_0} as the position of the first pixel in the assumed row of the image and @mymath{L} as the width of the image along that row. The units of @mymath{l_0} and @mymath{L} can be in any spatial units (for example meters) or an angular unit (like radians) multiplied by a fixed distance which is more common. To approximate @mymath{f(l)} over this interval, we need to find a set of frequencies and their corresponding `magnitude's (see @ref{Circles and the complex plane}). Therefore our aim is to show @mymath{f(l)} as the following sum of periodic functions: @dispmath{ f(l)=\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}n\over L}l} } @noindent Note that the different frequencies (@mymath{2{\pi}n/L}, in units of cycles per meters for example) are not arbitrary. They are all integer multiples of the fundamental frequency of @mymath{\omega_0=2\pi/L}. Recall that @mymath{L} was the length of the signal we want to model. Therefore, we see that the smallest possible frequency (or the frequency resolution) in the end, depends on the length we observed the signal or @mymath{L}. In the case of each dimension on an image, this is the size of the image in the respective dimension. The frequencies have been defined in this ``harmonic'' fashion to insure that the final sum is periodic outside of the @mymath{[l_0, l_0+L]} interval too. At this point, you might be thinking that the sky is not periodic with the same period as my camera's view angle. You are absolutely right! The important thing is that since your camera's observed region is the only region we are ``observing'' and will be using, the rest of the sky is irrelevant; so we can safely assume the sky is periodic outside of it. However, this working assumption will haunt us later in @ref{Edges in the frequency domain}. The frequencies are thus determined by definition. So all we need to do is to find the coefficients (@mymath{c_n}), or magnitudes, or radii of the circles for each frequency which is identified with the integer @mymath{n}. Fourier's approach was to multiply both sides with a fixed term: @dispmath{ f(l)e^{-i{2{\pi}m\over L}l}=\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}(n-m)\over L}l} } @noindent where @mymath{m>0}@footnote{ We could have assumed @mymath{m<0} and set the exponential to positive, but this is more clear.}. We can then integrate both sides over the observation period: @dispmath{ \int_{l_0}^{l_0+L}f(l)e^{-i{2{\pi}m\over L}l}dl =\int_{l_0}^{l_0+L}\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}(n-m)\over L}l}dl=\displaystyle\sum_{n=-\infty}^{\infty}c_n\int_{l_0}^{l_0+L}e^{i{2{\pi}(n-m)\over L}l}dl } @noindent Both @mymath{n} and @mymath{m} are positive integers. Also, we know that a complex exponential is periodic so after one period (@mymath{L}) it comes back to its starting point. Therefore @mymath{\int_{l_0}^{l_0+L}e^{2{\pi}k/L}dl=0} for any @mymath{k>0}. However, when @mymath{k=0}, this integral becomes: @mymath{\int_{l_0}^{l_0+T}e^0dt=\int_{l_0}^{l_0+T}dt=T}. Hence since the integral will be zero for all @mymath{n{\neq}m}, we get: @dispmath{ \displaystyle\sum_{n=-\infty}^{\infty}c_n\int_{l_0}^{l_0+T}e^{i{2{\pi}(n-m)\over L}l}dl=Lc_m } @noindent The origin of the axis is fundamentally an arbitrary position. So let's set it to the start of the image such that @mymath{l_0=0}. So we can find the ``magnitude'' of the frequency @mymath{2{\pi}m/L} within @mymath{f(l)} through the relation: @dispmath{ c_m={1\over L}\int_{0}^{L}f(l)e^{-i{2{\pi}m\over L}l}dl } @node Fourier transform, Dirac delta and comb, Fourier series, Frequency domain and Fourier operations @subsubsection Fourier transform In @ref{Fourier series}, we had to assume that the function is periodic outside of the desired interval with a period of @mymath{L}. Therefore, assuming that @mymath{L\rightarrow\infty} will allow us to work with any function. However, with this approximation, the fundamental frequency (@mymath{\omega_0}) or the frequency resolution that we discussed in @ref{Fourier series} will tend to zero: @mymath{\omega_0\rightarrow0}. In the equation to find @mymath{c_m}, every @mymath{m} represented a frequency (multiple of @mymath{\omega_0}) and the integration on @mymath{l} removes the dependence of the right side of the equation on @mymath{l}, making it only a function of @mymath{m} or frequency. Let's define the following two variables: @dispmath{\omega{\equiv}m\omega_0={2{\pi}m\over L}} @dispmath{F(\omega){\equiv}Lc_m} @noindent The equation to find the coefficients of each frequency in @ref{Fourier series} thus becomes: @dispmath{ F(\omega)=\int_{-\infty}^{\infty}f(l)e^{-i{\omega}l}dl. } @noindent The function @mymath{F(\omega)} is thus the @emph{Fourier transform} of @mymath{f(l)} in the frequency domain. So through this transformation, we can find (analyze) the magnitudes of the constituting frequencies or the value in the frequency space@footnote{As we discussed before, this `magnitude' can be interpreted as the radius of the circle rotating at this frequency in the epicyclic interpretation of the Fourier series, see @ref{epicycle} and @ref{iandtime}.} of our spatial input function. The great thing is that we can also do the reverse and later synthesize the input function from its Fourier transform. Let's do it: with the approximations above, multiply the right side of the definition of the Fourier Series (@ref{Fourier series}) with @mymath{1=L/L=({\omega_0}L)/(2\pi)}: @dispmath{ f(l)={1\over 2\pi}\displaystyle\sum_{n=-\infty}^{\infty}Lc_ne^{{2{\pi}in\over L}l}\omega_0={1\over 2\pi}\displaystyle\sum_{n=-\infty}^{\infty}F(\omega)e^{i{\omega}l}\Delta\omega } @noindent To find the right most side of this equation, we renamed @mymath{\omega_0} as @mymath{\Delta\omega} because it was our resolution, @mymath{2{\pi}n/L} was written as @mymath{\omega} and finally, @mymath{Lc_n} was written as @mymath{F(\omega)} as we defined above. Now, as @mymath{L\rightarrow\infty}, @mymath{\Delta\omega\rightarrow0} so we can write: @dispmath{ f(l)={1\over 2\pi}\int_{-\infty}^{\infty}F(\omega)e^{i{\omega}l}d\omega } Together, these two equations provide us with a very powerful set of tools that we can use to process (analyze) and recreate (synthesize) the input signal. Through the first equation, we can break up our input function into its constituent frequencies and analyze it, hence it is also known as @emph{analysis}. Using the second equation, we can synthesize or make the input function from the known frequencies and their magnitudes. Thus it is known as @emph{synthesis}. Here, we symbolize the Fourier transform (analysis) and its inverse (synthesis) of a function @mymath{f(l)} and its Fourier Transform @mymath{F(\omega)} as @mymath{{\cal F}[f]} and @mymath{{\cal F}^{-1}[F]}. @node Dirac delta and comb, Convolution theorem, Fourier transform, Frequency domain and Fourier operations @subsubsection Dirac delta and comb The Dirac @mymath{\delta} (delta) function (also known as an impulse) is the way that we convert a continuous function into a discrete one. It is defined to satisfy the following integral: @dispmath{\int_{-\infty}^{\infty}\delta(l)dl=1} @noindent When integrated with another function, it gives that function's value at @mymath{l=0}: @dispmath{\int_{-\infty}^{\infty}f(l)\delta(l)dt=f(0)} @noindent An impulse positioned at another point (say @mymath{l_0}) is written as @mymath{\delta(l-l_0)}: @dispmath{\int_{-\infty}^{\infty}f(l)\delta(l-l_0)dt=f(l_0)} @noindent The Dirac @mymath{\delta} function also operates similarly if we use summations instead of integrals. The Fourier transform of the delta function is: @dispmath{{\cal F}[\delta(l)]=\int_{-\infty}^{\infty}\delta(l)e^{-i{\omega}l}dl=e^{-i{\omega}0}=1} @dispmath{{\cal F}[\delta(l-l_0)]=\int_{-\infty}^{\infty}\delta(l-l_0)e^{-i{\omega}l}dl=e^{-i{\omega}l_0}} @noindent From the definition of the Dirac @mymath{\delta} we can also define a Dirac comb (@mymath{{\rm III}_P}) or an impulse train with infinite impulses separated by @mymath{P}: @dispmath{ {\rm III}_P(l)\equiv\displaystyle\sum_{k=-\infty}^{\infty}\delta(l-kP) } @noindent @mymath{P} is chosen to represent ``pixel width'' later in @ref{Sampling theorem}. Therefore the Dirac comb is periodic with a period of @mymath{P}. We have intentionally used a different name for the period of the Dirac comb compared to the input signal's length of observation that we showed with @mymath{L} in @ref{Fourier series}. This difference is highlighted here to avoid confusion later when these two periods are needed together in @ref{Discrete Fourier transform}. The Fourier transform of the Dirac comb will be necessary in @ref{Sampling theorem}, so let's derive it. By its definition, it is periodic, with a period of @mymath{P}, so the Fourier coefficients of its Fourier Series (@ref{Fourier series}) can be calculated within one period: @dispmath{{\rm III}_P=\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}n\over P}l}} @noindent We can now find the @mymath{c_n} from @ref{Fourier series}: @dispmath{ c_n={1\over P}\int_{-P/2}^{P/2}\delta(l)e^{-i{2{\pi}n\over P}l} ={1\over P}\quad\quad \rightarrow \quad\quad {\rm III}_P={1\over P}\displaystyle\sum_{n=-\infty}^{\infty}e^{i{2{\pi}n\over P}l} } @noindent So we can write the Fourier transform of the Dirac comb as: @dispmath{ {\cal F}[{\rm III}_P]=\int_{-\infty}^{\infty}{\rm III}_Pe^{-i{\omega}l}dl ={1\over P}\displaystyle\sum_{n=-\infty}^{\infty}\int_{-\infty}^{\infty}e^{-i(\omega-{2{\pi}n\over P})l}dl={1\over P}\displaystyle\sum_{n=-\infty}^{\infty}\delta\left(\omega-{2{\pi}n\over P}\right) } @noindent In the last step, we used the fact that the complex exponential is a periodic function, that @mymath{n} is an integer and that as we defined in @ref{Fourier transform}, @mymath{\omega{\equiv}m\omega_0}, where @mymath{m} was an integer. The integral will be zero for any @mymath{\omega} that is not equal to @mymath{2{\pi}n/P}, a more complete explanation can be seen in @ref{Fourier series}. Therefore, while in the spatial domain the impulses had spacing of @mymath{P} (meters for example), in the frequency space, the spacing between the different impulses are @mymath{2\pi/P} cycles per meters. @node Convolution theorem, Sampling theorem, Dirac delta and comb, Frequency domain and Fourier operations @subsubsection Convolution theorem The convolution (shown with the @mymath{\ast} operator) of the two functions @mymath{f(l)} and @mymath{h(l)} is defined as: @dispmath{ c(l)\equiv[f{\ast}h](l)=\int_{-\infty}^{\infty}f(\tau)h(l-\tau)d\tau } @noindent See @ref{Convolution process} for a more detailed physical (pixel based) interpretation of this definition. The Fourier transform of convolution (@mymath{C(\omega)}) can be written as: @dispmath{ C(\omega)=\int_{-\infty}^{\infty}[f{\ast}h](l)e^{-i{\omega}l}dl= \int_{-\infty}^{\infty}f(\tau)\left[\int_{-\infty}^{\infty}h(l-\tau)e^{-i{\omega}l}dl\right]d\tau } @noindent To solve the inner integral, let's define @mymath{s{\equiv}l-\tau}, so that @mymath{ds=dl} and @mymath{l=s+\tau} then the inner integral becomes: @dispmath{ \int_{-\infty}^{\infty}h(l-\tau)e^{-i{\omega}l}dl= \int_{-\infty}^{\infty}h(s)e^{-i{\omega}(s+\tau)}ds=e^{-i{\omega}\tau}\int_{-\infty}^{\infty}h(s)e^{-i{\omega}s}ds=H(\omega)e^{-i{\omega}\tau} } @noindent where @mymath{H(\omega)} is the Fourier transform of @mymath{h(l)}. Substituting this result for the inner integral above, we get: @dispmath{ C(\omega)=H(\omega)\int_{-\infty}^{\infty}f(\tau)e^{-i{\omega}\tau}d\tau=H(\omega)F(\omega)=F(\omega)H(\omega) } @noindent where @mymath{F(\omega)} is the Fourier transform of @mymath{f(l)}. So multiplying the Fourier transform of two functions individually, we get the Fourier transform of their convolution. The convolution theorem also proves a relation between the convolutions in the frequency space. Let's define: @dispmath{D(\omega){\equiv}F(\omega){\ast}H(\omega)} @noindent Applying the inverse Fourier Transform or synthesis equation (@ref{Fourier transform}) to both sides and following the same steps above, we get: @dispmath{d(l)=f(l)h(l)} @noindent Where @mymath{d(l)} is the inverse Fourier transform of @mymath{D(\omega)}. We can therefore re-write the two equations above formally as the convolution theorem: @dispmath{ {\cal F}[f{\ast}h]={\cal F}[f]{\cal F}[h] } @dispmath{ {\cal F}[fh]={\cal F}[f]\ast{\cal F}[h] } Besides its usefulness in blurring an image by convolving it with a given kernel, the convolution theorem also enables us to do another very useful operation in data analysis: to match the blur (or PSF) between two images taken with different telescopes/cameras or under different atmospheric conditions. This process is also known as de-convolution. Let's take @mymath{f(l)} as the image with a narrower PSF (less blurry) and @mymath{c(l)} as the image with a wider PSF which appears more blurred. Also let's take @mymath{h(l)} to represent the kernel that should be convolved with the sharper image to create the more blurry image. Above, we proved the relation between these three images through the convolution theorem. But there, we assumed that @mymath{f(l)} and @mymath{h(l)} are known (given) and the convolved image is desired. In de-convolution, we have @mymath{f(l)} --the sharper image-- and @mymath{f*h(l)} --the more blurry image-- and we want to find the kernel @mymath{h(l)}. The solution is a direct result of the convolution theorem: @dispmath{ {\cal F}[h]={{\cal F}[f{\ast}h]\over {\cal F}[f]} \quad\quad {\rm or} \quad\quad h(l)={\cal F}^{-1}\left[{{\cal F}[f{\ast}h]\over {\cal F}[f]}\right] } While this works really nice, it has two problems: @itemize @item If @mymath{{\cal F}[f]} has any zero values, then the inverse Fourier transform will not be a number! @item If there is significant noise in the image, then the high frequencies of the noise are going to significantly reduce the quality of the final result. @end itemize A standard solution to both these problems is the Weiner de-convolution algorithm@footnote{@url{https://en.wikipedia.org/wiki/Wiener_deconvolution}}. @node Sampling theorem, Discrete Fourier transform, Convolution theorem, Frequency domain and Fourier operations @subsubsection Sampling theorem Our mathematical functions are continuous, however, our data collecting and measuring tools are discrete. Here we want to give a mathematical formulation for digitizing the continuous mathematical functions so that later, we can retrieve the continuous function from the digitized recorded input. Assuming that we have a continuous function @mymath{f(l)}, then we can define @mymath{f_s(l)} as the `sampled' @mymath{f(l)} through the Dirac comb (see @ref{Dirac delta and comb}): @dispmath{ f_s(l)=f(l){\rm III}_P=\displaystyle\sum_{n=-\infty}^{\infty}f(l)\delta(l-nP) } @noindent The discrete data-element @mymath{f_k} (for example, a pixel in an image), where @mymath{k} is an integer, can thus be represented as: @dispmath{f_k=\int_{-\infty}^{\infty}f_s(l)dl=\int_{-\infty}^{\infty}f(l)\delta(l-kP)dt=f(kP)} Note that in practice, our discrete data points are not found in this fashion. Each detector pixel (in an image for example) has an area and averages the signal it receives over that area, not a mathematical point as the Dirac @mymath{\delta} function defines. However, as long as the variation in the signal over one detector pixel is not significant, this can be a good approximation. Having put this issue to the side, we can now try to find the relation between the Fourier transforms of the un-sampled @mymath{f(l)} and the sampled @mymath{f_s(l)}. For a more clear notation, let's define: @dispmath{F_s(\omega)\equiv{\cal F}[f_s]} @dispmath{D(\omega)\equiv{\cal F}[{\rm III}_P]} @noindent Then using the Convolution theorem (see @ref{Convolution theorem}), @mymath{F_s(\omega)} can be written as: @dispmath{F_s(\omega)={\cal F}[f(l){\rm III}_P]=F(\omega){\ast}D(\omega)} @noindent Finally, from the definition of convolution and the Fourier transform of the Dirac comb (see @ref{Dirac delta and comb}), we get: @dispmath{ \eqalign{ F_s(\omega) &= \int_{-\infty}^{\infty}F(\omega)D(\omega-\mu)d\mu \cr &= {1\over P}\displaystyle\sum_{n=-\infty}^{\infty}\int_{-\infty}^{\infty}F(\omega)\delta\left(\omega-\mu-{2{\pi}n\over P}\right)d\mu \cr &= {1\over P}\displaystyle\sum_{n=-\infty}^{\infty}F\left( \omega-{2{\pi}n\over P}\right).\cr } } @mymath{F(\omega)} was only a simple function, see @ref{samplingfreq}(left). However, from the sampled Fourier transform function we see that @mymath{F_s(\omega)} is the superposition of infinite copies of @mymath{F(\omega)} that have been shifted, see @ref{samplingfreq}(right). From the equation, it is clear that the shift in each copy is @mymath{2\pi/P}. @float Figure,samplingfreq @image{gnuastro-figures/samplingfreq, 15.2cm, , } @caption{Sampling causes infinite repetition in the frequency domain. FT is an abbreviation for `Fourier transform'. @mymath{\omega_m} represents the maximum frequency present in the input. @mymath{F(\omega)} is only symmetric on both sides of 0 when the input is real (not complex). In general @mymath{F(\omega)} is complex and thus cannot be simply plotted like this. Here we have assumed a real Gaussian @mymath{f(t)} which has produced a Gaussian @mymath{F(\omega)}.} @end float The input @mymath{f(l)} can have any distribution of frequencies in it. In the example of @ref{samplingfreq}(left), the input consisted of a range of frequencies equal to @mymath{\Delta\omega=2\omega_m}. Fortunately as @ref{samplingfreq}(right) shows, the assumed pixel size (@mymath{P}) we used to sample this hypothetical function was such that @mymath{2\pi/P>\Delta\omega}. The consequence is that each copy of @mymath{F(\omega)} has become completely separate from the surrounding copies. Such a digitized (sampled) data set is thus called @emph{over-sampled}. When @mymath{2\pi/P=\Delta\omega}, @mymath{P} is just small enough to finely separate even the largest frequencies in the input signal and thus it is known as @emph{critically-sampled}. Finally if @mymath{2\pi/P<\Delta\omega} we are dealing with an @emph{under-sampled} data set. In an under-sampled data set, the separate copies of @mymath{F(\omega)} are going to overlap and this will deprive us of recovering high constituent frequencies of @mymath{f(l)}. The effects of under-sampling in an image with high rates of change (for example a brick wall imaged from a distance) can clearly be visually seen and is known as @emph{aliasing}. When the input @mymath{f(l)} is composed of a finite range of frequencies, @mymath{f(l)} is known as a @emph{band-limited} function. The example in @ref{samplingfreq}(left) was a nice demonstration of such a case: for all @mymath{\omega<-\omega_m} or @mymath{\omega>\omega_m}, we have @mymath{F(\omega)=0}. Therefore, when the input function is band-limited and our detector's pixels are placed such that we have critically (or over-) sampled it, then we can exactly reproduce the continuous @mymath{f(l)} from the discrete or digitized samples. To do that, we just have to isolate one copy of @mymath{F(\omega)} from the infinite copies and take its inverse Fourier transform. This ability to exactly reproduce the continuous input from the sampled or digitized data leads us to the @emph{sampling theorem} which connects the inherent property of the continuous signal (its maximum frequency) to that of the detector (the spacing between its pixels). The sampling theorem states that the full (continuous) signal can be recovered when the pixel size (@mymath{P}) and the maximum constituent frequency in the signal (@mymath{\omega_m}) have the following relation@footnote{This equation is also shown in some places without the @mymath{2\pi}. Whether @mymath{2\pi} is included or not depends on how you define the frequency}: @dispmath{{2\pi\over P}>2\omega_m} @noindent This relation was first formulated by Harry Nyquist (1889 -- 1976 A.D.) in 1928 and formally proved in 1949 by Claude E. Shannon (1916 -- 2001 A.D.) in what is now known as the Nyquist-Shannon sampling theorem. In signal processing, the signal is produced (synthesized) by a transmitter and is received and de-coded (analyzed) by a receiver. Therefore producing a band-limited signal is necessary. In astronomy, we do not produce the shapes of our targets, we are only observers. Galaxies can have any shape and size, therefore ideally, our signal is not band-limited. However, since we are always confined to observing through an aperture, the aperture will cause a point source (for which @mymath{\omega_m=\infty}) to be spread over several pixels. This spread is quantitatively known as the point spread function or PSF. This spread does blur the image which is undesirable; however, for this analysis it produces the positive outcome that there will be a finite @mymath{\omega_m}. Though we should caution that any detector will have noise which will add lots of very high frequency (ideally infinite) changes between the pixels. However, the coefficients of those noise frequencies are usually exceedingly small. @node Discrete Fourier transform, Fourier operations in two dimensions, Sampling theorem, Frequency domain and Fourier operations @subsubsection Discrete Fourier transform As we have stated several times so far, the input image is a digitized, pixelated or discrete array of values (@mymath{f_s(l)}, see @ref{Sampling theorem}). The input is not a continuous function. Also, all our numerical calculations can only be done on a sampled, or discrete Fourier transform. Note that @mymath{F_s(\omega)} is not discrete, it is continuous. One way would be to find the analytic @mymath{F_s(\omega)}, then sample it at any desired ``freq-pixel''@footnote{We are using the made-up word ``freq-pixel'' so they are not confused with spatial domain ``pixels''.} spacing. However, this process would involve two steps of operations and computers in particular are not too good at analytic operations for the first step. So here, we will derive a method to directly find the `freq-pixel'ated @mymath{F_s(\omega)} from the pixelated @mymath{f_s(l)}. Let's start with the definition of the Fourier transform (see @ref{Fourier transform}): @dispmath{F_s(\omega)=\int_{-\infty}^{\infty}f_s(l)e^{-i{\omega}l}dl } @noindent From the definition of @mymath{f_s(\omega)} (using @mymath{x} instead of @mymath{n}) we get: @dispmath{ \eqalign{ F_s(\omega) &= \displaystyle\sum_{x=-\infty}^{\infty} \int_{-\infty}^{\infty}f(l)\delta(l-xP)e^{-i{\omega}l}dl \cr &= \displaystyle\sum_{x=-\infty}^{\infty} f_xe^{-i{\omega}xP} } } @noindent Where @mymath{f_x} is the value of @mymath{f(l)} on the point @mymath{x} or the value of the @mymath{x}th pixel. As shown in @ref{Sampling theorem} this function is infinitely periodic with a period of @mymath{2\pi/P}. So all we need is the values within one period: @mymath{0<\omega<2\pi/P}, see @ref{samplingfreq}. We want @mymath{X} samples within this interval, so the frequency difference between each frequency sample or freq-pixel is @mymath{1/XP}. Hence we will evaluate the equation above on the points at: @dispmath{\omega={u\over XP} \quad\quad u = 0, 1, 2, ..., X-1} @noindent Therefore the value of the freq-pixel @mymath{u} in the frequency domain is: @dispmath{F_u=\displaystyle\sum_{x=0}^{X-1} f_xe^{-i{ux\over X}} } @noindent Therefore, we see that for each freq-pixel in the frequency domain, we are going to need all the pixels in the spatial domain@footnote{So even if one pixel is a blank pixel (see @ref{Blank pixels}), all the pixels in the frequency domain will also be blank.}. If the input (spatial) pixel row is also @mymath{X} pixels wide, then we can exactly recover the @mymath{x}th pixel with the following summation: @dispmath{f_x={1\over X}\displaystyle\sum_{u=0}^{X-1} F_ue^{i{ux\over X}} } When the input pixel row (we are still only working on 1D data) has @mymath{X} pixels, then it is @mymath{L=XP} spatial units wide. @mymath{L}, or the length of the input data was defined in @ref{Fourier series} and @mymath{P} or the space between the pixels in the input was defined in @ref{Dirac delta and comb}. As we saw in @ref{Sampling theorem}, the input (spatial) pixel spacing (@mymath{P}) specifies the range of frequencies that can be studied and in @ref{Fourier series} we saw that the length of the (spatial) input, (@mymath{L}) determines the resolution (or size of the freq-pixels) in our discrete Fourier transformed image. Both result from the fact that the frequency domain is the inverse of the spatial domain. @node Fourier operations in two dimensions, Edges in the frequency domain, Discrete Fourier transform, Frequency domain and Fourier operations @subsubsection Fourier operations in two dimensions Once all the relations in the previous sections have been clearly understood in one dimension, it is very easy to generalize them to two or even more dimensions since each dimension is by definition independent. Previously we defined @mymath{l} as the continuous variable in 1D and the inverse of the period in its direction to be @mymath{\omega}. Let's show the second spatial direction with @mymath{m} the the inverse of the period in the second dimension with @mymath{\nu}. The Fourier transform in 2D (see @ref{Fourier transform}) can be written as: @dispmath{F(\omega, \nu)=\int_{-\infty}^{\infty}\int_{-\infty}^{\infty} f(l, m)e^{-i({\omega}l+{\nu}m)}dl} @dispmath{f(l, m)=\int_{-\infty}^{\infty}\int_{-\infty}^{\infty} F(\omega, \nu)e^{i({\omega}l+{\nu}m)}dl} The 2D Dirac @mymath{\delta(l,m)} is non-zero only when @mymath{l=m=0}. The 2D Dirac comb (or Dirac brush! See @ref{Dirac delta and comb}) can be written in units of the 2D Dirac @mymath{\delta}. For most image detectors, the sides of a pixel are equal in both dimensions. So @mymath{P} remains unchanged, if a specific device is used which has non-square pixels, then for each dimension a different value should be used. @dispmath{{\rm III}_P(l, m)\equiv\displaystyle\sum_{j=-\infty}^{\infty} \displaystyle\sum_{k=-\infty}^{\infty} \delta(l-jP, m-kP) } The Two dimensional Sampling theorem (see @ref{Sampling theorem}) is thus very easily derived as before since the frequencies in each dimension are independent. Let's take @mymath{\nu_m} as the maximum frequency along the second dimension. Therefore the two dimensional sampling theorem says that a 2D band-limited function can be recovered when the following conditions hold@footnote{If the pixels are not a square, then each dimension has to use the respective pixel size, but since most imagers have square pixels, we assume so here too}: @dispmath{ {2\pi\over P} > 2\omega_m \quad\quad\quad {\rm and} \quad\quad\quad {2\pi\over P} > 2\nu_m} Finally, let's represent the pixel counter on the second dimension in the spatial and frequency domains with @mymath{y} and @mymath{v} respectively. Also let's assume that the input image has @mymath{Y} pixels on the second dimension. Then the two dimensional discrete Fourier transform and its inverse (see @ref{Discrete Fourier transform}) can be written as: @dispmath{F_{u,v}=\displaystyle\sum_{x=0}^{X-1}\displaystyle\sum_{y=0}^{Y-1} f_{x,y}e^{-i({ux\over X}+{vy\over Y})} } @dispmath{f_{x,y}={1\over XY}\displaystyle\sum_{u=0}^{X-1}\displaystyle\sum_{v=0}^{Y-1} F_{u,v}e^{i({ux\over X}+{vy\over Y})} } @node Edges in the frequency domain, , Fourier operations in two dimensions, Frequency domain and Fourier operations @subsubsection Edges in the frequency domain With a good grasp of the frequency domain, we can revisit the problem of convolution on the image edges, see @ref{Edges in the spatial domain}. When we apply the convolution theorem (see @ref{Convolution theorem}) to convolve an image, we first take the discrete Fourier transforms (DFT, @ref{Discrete Fourier transform}) of both the input image and the kernel, then we multiply them with each other and then take the inverse DFT to construct the convolved image. Of course, in order to multiply them with each other in the frequency domain, the two images have to be the same size, so let's assume that we pad the kernel (it is usually smaller than the input image) with zero valued pixels in both dimensions so it becomes the same size as the input image before the DFT. Having multiplied the two DFTs, we now apply the inverse DFT which is where the problem is usually created. If the DFT of the kernel only had values of 1 (unrealistic condition!) then there would be no problem and the inverse DFT of the multiplication would be identical with the input. However in real situations, the kernel's DFT has a maximum of 1 (because the sum of the kernel has to be one, see @ref{Convolution process}) and decreases something like the hypothetical profile of @ref{samplingfreq}. So when multiplied with the input image's DFT, the coefficients or magnitudes (see @ref{Circles and the complex plane}) of the smallest frequency (or the sum of the input image pixels) remains unchanged, while the magnitudes of the higher frequencies are significantly reduced. As we saw in @ref{Sampling theorem}, the Fourier transform of a discrete input will be infinitely repeated. In the final inverse DFT step, the input is in the frequency domain (the multiplied DFT of the input image and the kernel DFT). So the result (our output convolved image) will be infinitely repeated in the spatial domain. In order to accurately reconstruct the input image, we need all the frequencies with the correct magnitudes. However, when the magnitudes of higher frequencies are decreased, longer periods (shorter frequencies) will dominate in the reconstructed pixel values. Therefore, when constructing a pixel on the edge of the image, the newly empowered longer periods will look beyond the input image edges and will find the repeated input image there. So if you convolve an image in this fashion using the convolution theorem, when a bright object exists on one edge of the image, its blurred wings will be present on the other side of the convolved image. This is often termed as circular convolution or cyclic convolution. So as long as we are dealing with convolution in the frequency domain, there is nothing we can do about the image edges. The least we can do is to eliminate the ghosts of the other side of the image. So, we add zero valued pixels to both the input image and the kernel in both dimensions so the image that will be convolved has the a size equal to the sum of both images in each dimension. Of course, the effect of this zero-padding is that the sides of the output convolved image will become dark. To put it another way, the edges are going to drain the flux from nearby objects. But at least it is consistent across all the edges of the image and is predictable. In Convolve, you can see the padded images when inspecting the frequency domain convolution steps with the @option{--viewfreqsteps} option. @node Spatial vs. Frequency domain, Convolution kernel, Frequency domain and Fourier operations, Convolve @subsection Spatial vs. Frequency domain With the discussions above it might not be clear when to choose the spatial domain and when to choose the frequency domain. Here we will try to list the benefits of each. @noindent The spatial domain, @itemize @item Can correct for the edge effects of convolution, see @ref{Edges in the spatial domain}. @item Can operate on blank pixels. @item Can be faster than frequency domain when the kernel is small (in terms of the number of pixels on the sides). @end itemize @noindent The frequency domain, @itemize @item Will be much faster when the image and kernel are both large. @end itemize @noindent As a general rule of thumb, when working on an image of modeled profiles use the frequency domain and when working on an image of real (observed) objects use the spatial domain (corrected for the edges). The reason is that if you apply a frequency domain convolution to a real image, you are going to loose information on the edges and generally you don't want large kernels. But when you have made the profiles in the image yourself, you can just make a larger input image and crop the central parts to completely remove the edge effect, see @ref{If convolving afterwards}. Also due to oversampling, both the kernels and the images can become very large and the speed boost of frequency domain convolution will significantly improve the processing time, see @ref{Oversampling}. @node Convolution kernel, Invoking astconvolve, Spatial vs. Frequency domain, Convolve @subsection Convolution kernel All the programs that need convolution will need to be given a convolution kernel file and extension. In most cases (other than Convolve, see @ref{Convolve}) the kernel file name is optional. However, the extension is necessary and must be specified either on the command-line or at least one of the configuration files (see @ref{Configuration files}). Within Gnuastro, there are two ways to create a kernel image: @itemize @item MakeProfiles: You can use MakeProfiles to create a parametric (based on a radial function) kernel, see @ref{MakeProfiles}. By default MakeProfiles will make the Gaussian and Moffat profiles in a separate file so you can feed it into any of the programs. @item ConvertType: You can write your own desired kernel into a text file table and convert it to a FITS file with ConvertType, see @ref{ConvertType}. Just be careful that the kernel has to have an odd number of pixels along its two axes, see @ref{Convolution process}. All the programs that do convolution will normalize the kernel internally, so if you choose this option, you don't have to worry about normalizing the kernel. Only within Convolve, there is an option to disable normalization, see @ref{Invoking astconvolve}. @end itemize @noindent The two options to specify a kernel file name and its extension are shown below. These are common between all the programs that will do convolution. @table @option @item -k @itemx --kernel (@option{=STR}) The convolution kernel file name. The @code{BITPIX} (data type) value of this file can be any standard type and it does not necessarily have to be normalized. Several operations will be done on the kernel image prior to the program's processing: @itemize @item It will be converted to floating point type. @item All blank pixels (see @ref{Blank pixels}) will be set to zero. @item It will be normalized so the sum of its pixels equal unity. @item It will be flipped so the convolved image has the same orientation. This is only relevant if the kernel is not circular. See @ref{Convolution process}. @end itemize @item -U @itemx --khdu (@option{=STR}) The convolution kernel HDU. Although the kernel file name is optional, before running any of the programs, they need to have a value for @option{--khdu} even if the default kernel is to be used. So be sure to keep its value in at least one of the configuration files (see @ref{Configuration files}). By default, the system configuration file has a value. @item --fullconvolution Ignore the (possible) channels in the mesh grid when doing spatial convolution, see @ref{Tiling an image}. When applied over a mesh grid, spatial convolution will be done independently on each channel. This is necessary when the noise properties of each channel are different and so the pixels should not be mixed. With this option, all channel information is going to be ignored. Currently this option is not deployed for the frequency space convolutions. @end table @node Invoking astconvolve, , Convolution kernel, Convolve @subsection Invoking Convolve Convolve an input image with a known kernel. The general template for Convolve is: @example $ astconvolve [OPTION...] ASTRdata @end example @noindent One line examples: @example $ astconvolve --kernel=psf.fits mockimg.fits $ astconvolve --kernel=sharperimage.fits --makekernel\ blurryimage.fits @end example The only argument accepted by Convolve is an input image file. Some of the options are the same between Convolve and some other Gnuastro programs. Therefore, to avoid repetition, they will not be repeated here. For the full list of options shared by all Gnuastro programs, please see @ref{Common options}. @ref{Mesh grid options} lists all the options related to specifying a mesh grid which is currently only used in spatial convolution. Note that here, no interpolation or smoothing is defined, only channels and the mesh size are important. @ref{Convolution kernel} lists the the convolution kernel options. It is also possible to specify a mask image for the input. In that case, see @ref{Mask image}. Here we will only explain the options particular to Convolve. Run Convolve with @option{--help} in order to see the full list of options Convolve accepts, irrespective of where they are explained in this book. @table @option @item --nokernelflip Do not flip the kernel after reading it the spatial domain convolution. This can be useful if the flipping has already been applied to the kernel. @item --nokernelnorm Do not normalize the kernel after reading it, such that the sum of its pixels is unity. @item -f @itemx --frequency @cindex Discrete Fourier transform Convolve using discrete Fourier transform in the frequency domain: The Fourier transform of both arrays is first calculated and multiplied. Then the inverse Fourier transform is applied to the product to give the final convolved image. For large images, this process will be more efficient than convolving in the spatial domain. However, the edges of the image will loose some flux, see @ref{Edges in the spatial domain}. @item -p @itemx --spatial Convolve in the spatial domain, see @ref{Convolution process}. @item --viewfreqsteps With this option a file with the initial name of the output file will be created that is suffixed with @file{_freqsteps.fits}, all the steps done to arrive at the final convolved image are saved as extensions in this file. The extensions in order are: @enumerate @item The padded input image. In frequency domain convolution the two images (input and convolved) have to be the same size and both should be padded by zeros. @item The padded kernel, similar to the above. @item @cindex Phase angle @cindex Complex numbers @cindex Numbers, complex @cindex Fourier spectrum @cindex Spectrum, Fourier The Fourier spectrum of the forward Fourier transform of the input image. Note that the Fourier transform is a complex operation (and not view able in one image!) So we either have to show the `Fourier spectrum' or the `Phase angle'. For the complex number @mymath{a+ib}, the Fourier spectrum is defined as @mymath{\sqrt{a^2+b^2}} while the phase angle is defined as @mymath{\arctan(b/a)}. @item The Fourier spectrum of the forward Fourier transform of the kernel image. @item The Fourier spectrum of the multiplied (through complex arithmetic) transformed images. @item @cindex Round-off error @cindex Floating point round-off error @cindex Error, floating point round-off The inverse Fourier transform of the multiplied image. If you open it, you will see that the convolved image is now in the center, not on one side of the image as it started with (in the padded image of the first extension). If you are working on a mock image which originally had pixels of precisely 0.0, you will notice that in those parts that your convolved profile(s) did not convert, the values are now @mymath{\sim10^{-18}}, this is due to floating-point round off errors. Therefore in the final step (when cropping the central parts of the image), we also remove any pixel with a value less than @mymath{10^{-17}}. @end enumerate @item -m @itemx --makekernel (@option{=INT}) If this option is called, Convolve will do de-convolution (see @ref{Convolution theorem}). The image specified by the @option{--kernel} option is assumed to be the sharper (less blurry) image and the input image is assumed to be the more blurry image. The two images have to be the same size. Some notes to take into account for a good result: Noise has large frequencies which can make the result less reliable for the higher frequencies of the kernel. So all the frequencies which have a spectrum smaller than 0.005 in the frequency domain are set to zero and not divided. This will cause the wings of the final kernel to be flatter than they would ideally be which will make the convolved image result unreliable. The value given to this option will be used as the maximum radius of the kernel. Any pixel in the final kernel that is larger than this distance from the center will be set to zero. @itemize @item Choose a bright (unsaturated) star and use a region box (with ImageCrop for example, see @ref{ImageCrop}) that is sufficiently above the noise. @item Use ImageWarp (see @ref{ImageWarp}) to warp the pixel grid so the star's center is exactly on the center of the central pixel in the cropped image. This will certainly slightly degrade the result, however, it is necessary. If there are multiple good stars, you can shift all of them, then normalize them (so the sum of each star's pixels is one) and then take their average to decrease this effect. @item The shifting might move the center of the star by one pixel in any direction, so crop the central pixel of the warped image to have a clean image for the de-convolution. @end itemize @end table @node ImageWarp, SubtractSky, Convolve, Image manipulation @section ImageWarp Image warping is the process of mapping the pixels of one image onto a new pixel grid. This process is sometimes known as transformation, however following the discussion of Heckbert 1989@footnote{Paul S. Heckbert. 1989. @emph{Fundamentals of Texture mapping and Image Warping}, Master's thesis at University of California, Berkely.} we will not be using that term because it can be confused with only pixel value or flux transformations. Here we specifically mean the pixel grid transformation which is better conveyed with `warp'. @cindex Gravitational lensing Image wrapping is a very important step in astronomy, both in observational data analysis and in simulating modeled images. In modeling, warping an image is necessary when we want to apply grid transformations to the initial models, for example in simulating gravitational lensing (Radial warpings are not yet included in ImageWarp). Observational reasons for warping an image are listed below: @itemize @cindex Signal to noise ratio @item @strong{Noise:} Most scientifically interesting targets are inherently faint (have a very low Signal to noise ratio). Therefore one short exposure is not enough to detect such objects that are drowned deeply in the noise. We need multiple exposures so we can add them together and increase the objects' signal to noise ratio. Keeping the telescope fixed on one field of the sky is practically impossible. Therefore very deep observations have to put into the same grid before adding them. @cindex Mosaicing @cindex Image mosaic @item @strong{Resolution:} If we have multiple images of one patch of the sky (hopefully at multiple orientations) we can warp them to the same grid. The multiple orientations will allow us to `guess' the values of pixels on an output pixel grid that has smaller pixel sizes and thus increase the resolution of the output. This process of merging multiple observations is known as Mosaicing. @cindex Cosmic rays @item @strong{Cosmic rays:} Cosmic rays can randomly fall on any part of an image. If they collide vertically with the camera, they are going to create a very sharp and bright spot that in most cases can be separated easily@footnote{All astronomical targets are blurred with the PSF, see @ref{PSF}, however a cosmic ray is not and so it is very sharp (it suddenly stops at one pixel).}. However, depending on the depth of the camera pixels, and the angle that a cosmic rays collides with it, it can cover a line-like larger area on the CCD which makes the detection using their sharp edges very hard and error prone. One of the best methods to remove cosmic rays is to compare multiple images of the same field. To do that, we need all the images to be on the same pixel grid. @cindex Optical distortion @cindex Distortion, optical @item @strong{Optical distortion:} (Not yet included in ImageWarp) In wide field images, the optical distortion that occurs on the outer parts of the focal plane will make accurate comparison of the objects at various locations impossible. It is therefore necessary to warp the image and correct for those distortions prior to the analysis. @cindex ACS @cindex CCD @cindex WFC3 @cindex Wide Field Camera 3 @cindex Charge-coupled device @cindex Hubble Space Telescope @cindex Advanced camera for surveys @item @strong{Detector not on focal plane:} In some cases (like the Hubble Space Telescope ACS and WFC3 cameras), the CCD might be tilted compared to the focal plane, therefore the recorded CCD pixels have to be projected onto the focal plane before further analysis. @end itemize @menu * Warping basics:: Basics of coordinate transformation. * Merging multiple warpings:: How to merge multiple matrices. * Resampling:: Warping an image is re-sampling it. * Invoking astimgwarp:: Arguments and options for ImageWarp. @end menu @node Warping basics, Merging multiple warpings, ImageWarp, ImageWarp @subsection Warping basics @cindex Scaling @cindex Coordinate transformation Let's take @mymath{\left[\matrix{u&v}\right]} as the coordinates of a point in the input image and @mymath{\left[\matrix{x&y}\right]} as the coordinates of that same point in the output image@footnote{These can be any real number, we are not necessarily talking about integer pixels here.}. The simplest form of coordinate transformation (or warping) is the scaling of the coordinates, let's assume we want to scale the first axis by @mymath{M} and the second by @mymath{N}, the output coordinates of that point can be calculated by @dispmath{\left[\matrix{x\cr y}\right]= \left[\matrix{Mu\cr Nv}\right]= \left[\matrix{M&0\cr0&N}\right]\left[\matrix{u\cr v}\right]} @cindex Matrix @cindex Multiplication, Matrix @cindex Rotation of coordinates @noindent Note that these are matrix multiplications. We thus see that we can represent any such grid warping as a matrix. Another thing we can do with this @mymath{2\times2} matrix is to rotate the output coordinate around the common center of both coordinates. If the output is rotated anticlockwise by @mymath{\theta} degrees from the positive (to the right) horizontal axis, then the warping matrix should become: @dispmath{\left[\matrix{x\cr y}\right]= \left[\matrix{ucos\theta-vsin\theta\cr usin\theta+vcos\theta}\right]= \left[\matrix{cos\theta&-sin\theta\cr sin\theta&cos\theta}\right] \left[\matrix{u\cr v}\right] } @cindex Flip coordinates @noindent We can also flip the coordinates around the first axis, the second axis and the coordinate center with the following three matrices respectively: @dispmath{\left[\matrix{1&0\cr0&-1}\right]\quad\quad \left[\matrix{-1&0\cr0&1}\right]\quad\quad \left[\matrix{-1&0\cr0&-1}\right]} @cindex Shear @noindent The final thing we can do with this definition of a @mymath{2\times2} warping matrix is shear. If we want the output to be sheared along the first axis with @mymath{A} and along the second with @mymath{B}, then we can use the matrix: @dispmath{\left[\matrix{1&A\cr B&1}\right]} @noindent To have one matrix representing any combination of these steps, you use matrix multiplication, see @ref{Merging multiple warpings}. So any combinations of these transformations can be displayed with one @mymath{2\times2} matrix: @dispmath{\left[\matrix{a&b\cr c&d}\right]} @cindex Wide Field Camera 3 @cindex Hubble Space Telescope @cindex Advanced Camera for Surveys The transformations above can cover a lot of the needs of most coordinate transformations. However they are limited to mapping the point @mymath{[\matrix{0&0}]} to @mymath{[\matrix{0&0}]}. Therefore they are useless if you want one coordinate to be shifted compared to the other one. They are also space invariant, meaning that all the coordinates in the image will receive the same transformation. In other words, all the pixels in the output image will have the same area if placed over the input image. So transformations which require varying output pixel sizes like projections cannot be applied through this @mymath{2\times2} matrix either (for example for the tilted ACS and WFC3 camera detectors on board the Hubble space telescope). @cindex M@"obius, August. F. @cindex Homogeneous coordinates @cindex Coordinates, homogeneous To add these further capabilities, namely translation and projection, we use the homogeneous coordinates. They were defined about 200 years ago by August Ferdinand M@"obius (1790 -- 1868). For simplicity, we will only discuss points on a 2D plane and avoid the complexities of higher dimensions. We cannot provide a deep mathematical introduction here, interested readers can get a more detailed explanation from Wikipedia@footnote{@url{http://en.wikipedia.org/wiki/Homogeneous_coordinates}} and the references therein. By adding an extra coordinate to a point we can add the flexibility we need. The point @mymath{[\matrix{x&y}]} can be represented as @mymath{[\matrix{xZ&yZ&Z}]} in homogeneous coordinates. Therefore multiplying all the coordinates of a point in the homogeneous coordinates with a constant will give the same point. Put another way, the point @mymath{[\matrix{x&y&Z}]} corresponds to the point @mymath{[\matrix{x/Z&y/Z}]} on the constant @mymath{Z} plane. Setting @mymath{Z=1}, we get the input image plane, so @mymath{[\matrix{u&v&1}]} corresponds to @mymath{[\matrix{u&v}]}. With this definition, the transformations above can be generally written as: @dispmath{\left[\matrix{x\cr y\cr 1}\right]= \left[\matrix{a&b&0\cr c&d&0\cr 0&0&1}\right] \left[\matrix{u\cr v\cr 1}\right]} @noindent @cindex Affine Transformation @cindex Transformation, affine We thus acquired 4 extra degrees of freedom. By giving non-zero values to the zero valued elements of the last column we can have translation (try the matrix multiplication!). In general, any coordinate transformation that is represented by the matrix below is known as an affine transformation@footnote{@url{http://en.wikipedia.org/wiki/Affine_transformation}}: @dispmath{\left[\matrix{a&b&c\cr d&e&f\cr 0&0&1}\right]} @cindex Homography @cindex Projective transformation @cindex Transformation, projective We can now consider translation, but the affine transform is still spatially invariant. Giving non-zero values to the other two elements in the matrix above gives us the projective transformation or Homography@footnote{@url{http://en.wikipedia.org/wiki/Homography}} which is the most general type of transformation with the @mymath{3\times3} matrix: @dispmath{\left[\matrix{x'\cr y'\cr w}\right]= \left[\matrix{a&b&c\cr d&e&f\cr g&h&1}\right] \left[\matrix{u\cr v\cr 1}\right]} @noindent So the output coordinates can be calculated from: @dispmath{x={x' \over w}={au+bv+c \over gu+hv+1}\quad\quad\quad\quad y={y' \over w}={du+ev+f \over gu+hv+1}} Thus with homography we can change the sizes of the output pixels on the input plane, giving a `perspective'-like visual impression. This can be quantitatively seen in the two equations above. When @mymath{g=h=0}, the denominator is independent of @mymath{u} or @mymath{v} and thus we have spatial invariance. Homography preserves lines at all orientations. A very useful fact about homography is that its inverse is also a homography. These two properties play a very important role in the implementation of this transformation. A short but instructive and illustrated review of affine, projective and also bi-linear mappings is provided in Heckbert 1989@footnote{Paul S. Heckbert. 1989. @emph{Fundamentals of Texture mapping and Image Warping}, Master's thesis at University of California, Berkely. Note that since points are defined as row vectors there, the matrix is the transpose of the one discussed here.}. @node Merging multiple warpings, Resampling, Warping basics, ImageWarp @subsection Merging multiple warpings @cindex Commutative property @cindex Matrix multiplication @cindex Multiplication, matrix @cindex Non-commutative operations @cindex Operations, non-commutative In @ref{Warping basics} we saw how one basic warping/transformation can be represented with a 3 by 3 matrix. To make more complex warpings these matrices have to be multiplied through matrix multiplication. However matrix multiplication is not commutative, so the order of the set of matrices you use for the multiplication is going to be very important. The first warping should be placed as the left-most matrix. The second warping to the right of that and so on. The second transformation is going to occur on the warped coordinates of the first. As an example for merging a few transforms into one matrix, the multiplication below represents the rotation of an image about a point @mymath{[\matrix{U&V}]} anticlockwise from the horizontal axis by an angle of @mymath{\theta}. To do this, first we take the origin to @mymath{[\matrix{U&V}]} through translation. Then we rotate the image, then we translate it back to where it was initially. These three operations can be merged in one operation by calculating the matrix multiplication below: @dispmath{\left[\matrix{1&0&U\cr0&1&V\cr{}0&0&1}\right] \left[\matrix{cos\theta&-sin\theta&0\cr sin\theta&cos\theta&0\cr 0&0&1}\right] \left[\matrix{1&0&-U\cr0&1&-V\cr{}0&0&1}\right]} @node Resampling, Invoking astimgwarp, Merging multiple warpings, ImageWarp @subsection Resampling @cindex Pixel @cindex Camera @cindex Detector @cindex Sampling @cindex Resampling @cindex Pixel mixing @cindex Photoelectrons @cindex Picture element @cindex Mixing pixel values A digital image is composed of discrete `picture elements' or `pixels'. When a real image is created from a camera or detector, each pixel's area is used to store the number of photo-electrons that were created when incident photons collided with that pixel's surface area. This process is called the `sampling' of a continuous or analog data into digital data. When we change the pixel grid of an image or warp it as we defined in @ref{Warping basics}, we have to `guess' the flux value of each pixel on the new grid based on the old grid, or re-sample it. Because of the `guessing', any form of warping on the data is going to degrade the image and mix the original pixel values with each other. So if an analysis can be done on an un-warped data image, it is best to leave the image untouched and pursue the analysis. However as discussed in @ref{ImageWarp} this is not possible most of the times, so we have to accept the problem and re-sample the image. @cindex Point pixels @cindex Interpolation @cindex Bicubic interpolation @cindex Signal to noise ratio @cindex Bi-linear interpolation @cindex Interpolation, bicubic @cindex Interpolation, bi-linear In most applications of image processing, it is sufficient to consider each pixel to be a point and not an area. This assumption can significantly speed up the processing of an image and also the simplicity of the code. It is a fine assumption when the signal to noise ratio of the objects are very large. The question will then be one of interpolation because you have multiple points distributed over the output image and you want to find the values at the pixel centers. To increase the accuracy, you might also sample more than one point from within a pixel giving you more points for a more accurate interpolation in the output grid. @cindex Image edges @cindex Edges, image However, interpolation has several problems. The first one is that it will depend on the type of function you want to assume for the interpolation. For example you can choose a bi-linear or bi-cubic (the `bi's are for the 2 dimensional nature of the data) interpolation method. For the latter there are various ways to set the constants@footnote{see @url{http://entropymine.com/imageworsener/bicubic/} for a nice introduction.}. Such functional interpolation functions can fail seriously on the edges of an image. They will also need normalization so that the flux of the objects before and after the warpings are comparable. The most basic problem with such techniques is that they are based on a point while a detector pixel is an area. They add a level of subjectivity to the data (make more assumptions through the functions than the data can handle). For most applications this is fine, but in scientific applications where detection of the faintest possible galaxies or fainter parts of bright galaxies is our aim, we cannot afford this loss. Because of these reasons ImageWarp will not use such interpolation techniques. @cindex Drizzle @cindex Pixel mixing @cindex Exact area resampling ImageWarp will do interpolation based on ``pixel mixing''@footnote{For a graphic demonstration see @url{http://entropymine.com/imageworsener/pixelmixing/}.} or ``area resampling''. This is also what the Hubble Space Telescope pipeline calls ``Drizzling''@footnote{@url{http://en.wikipedia.org/wiki/Drizzle_(image_processing)}}. This technique requires no functions, it is thus non-parametric. It is also the closest we can get (make least assumptions) to what actually happens on the detector pixels. The basic idea is that you reverse-transform each output pixel to find which pixels of the input image it covers and what fraction of the area of the input pixels are covered. To find the output pixel value, you simply sum the value of each input pixel weighted by the overlap fraction (between 0 to 1) of the output pixel and that input pixel. Through this process, pixels are treated as an area not as a point (which is how detectors create the image), also the brightness (see @ref{Flux Brightness and magnitude}) of an object will be left completely unchanged. If there are very high spatial-frequency signals in the image (for example fringes) which vary on a scale smaller than your output image pixel size, pixel mixing can cause ailiasing@footnote{@url{http://en.wikipedia.org/wiki/Aliasing}}. So if the input image has fringes, they have to be calculated and removed separately (which would naturally be done in any astronomical application). Because of the PSF no astronomical target has a sharp change in the signal so this issue is less important for astronomical applications, see @ref{PSF}. @node Invoking astimgwarp, , Resampling, ImageWarp @subsection Invoking ImageWarp The general template for invoking ImageWarp is: @example $ astimgwarp [OPTIONS...] [matrix.txt] InputImage @end example @noindent One line examples: @example $ astimgwarp matrix.txt image.fits $ astimgwarp --align rawimage.fits $ astimgwarp --scale 1.82 --translate 2.1 image.fits $ astimgwarp --rotate=37.92 --scale=0.8 image.fits $ astimgwarp --matrix=0.2,0,0.4,0,0.2,0.4,0,0,1 image.fits $ astimgwarp --matrix="0.7071,-0.7071 0.7071,0.7071" image.fits @end example ImageWarp can accept two arguments, one (an image) is mandatory if any processing is to be done. An optional argument is a plain text file, which must contain the warp/transform matrix, see @ref{Warping basics}. When this text file is specified, then all options related to the matrix will be ignored (see below for the options). The general options to all Gnuastro programs (including ImageWarp) can be seen in @ref{Common options}. To be the most accurate the input image will be converted to double precision floating points and all the processing will be done in this format. By default, in the end, the output image will be converted back to the input image data type. Note that if the input type was not a floating point format, then the floating point output pixels are going to be rounded to the nearest integer (using the @code{round} function in the C programming language) which can lead to a loss of data. This behavior can be disabled with the @option{--doubletype} option. The input file and input warping matrix elements are stored in the output's header. When using options, warps can be specified in a modular form, with options to specify each transformation (for example @option{--rotate}, or @option{--scale}), or directly as a matrix (with @option{--matrix}). If specified together, the latter (direct matrix) will take precedence and all the modular warpings will be ignored. Any number of modular warpings can be specified on the command-line and configuration files. If more than one modular warping is given, all will be merged to create one warping matrix. As described in @ref{Merging multiple warpings}, matrix multiplication is not commutative, so the order of specifying the modular warpings on the command-line, and/or configuration files makes a difference (see @ref{Configuration file precedence}). Below, the modular warpings are first listed (see @ref{Warping basics} for the definition of each type of warping), then the other ImageWarp options. @cindex FITS standard Based on the FITS standard, integer values are assigned to the center of a pixel and the coordinate [1.0, 1.0] is the center of the bottom left (first) image pixel. So the point [0.0, 0.0] is half a pixel away (in each axis) from the bottom left vertice of the first pixel. The resampling that is done in ImageWarp (see @ref{Resampling}) is dependent on this coordinate. So correction is done internally. With this resampling, the image must be warped relative to the bottom left vertice of the bottom left pixel and that point should lie at [0.0, 0.0]. So for a correct sampling, the warping center must first be translated by [0.5, 0.5], then the warp should be done and finally, a [-0.5, -0.5] translation should be specified. This correction is done internally in the following cases and can be disabled with the @option{--nofitscorrect} option. @itemize @item A 2D matrix is given in a file (as an argument). @item A 2D matrix is specified with the @option{--matrix} option. @item When modular warpings are used. @end itemize @table @option @item -a @itemx --align Align the image and celestial (WCS) axes, such that the vertical image direction (when viewed in SAO ds9) corresponds to the declination and the horizontal axis is the inverse of the Right Ascension (RA). The inverse of the RA is chosen so the image can correspond to what you would actually see on the sky and is common in most survey images. Align is internally treated just like a rotation (@option{--rotation}), but uses the input image's WCS to find the rotation angle. @item -r @itemx --rotate (@option{=FLT}) Rotate the input image by the given angle in degrees. Note that commonly, the WCS structure of the image is set such that the RA is the inverse of the image horizontal axis which increases towards the right in the FITS standard and as viewed by SAO ds9. So the default center for rotation is on the right of the image. If you want to rotate about other points, you have to translate the warping center first (with @option{--translate}) then apply your rotation and then return the center back to the original position (with another call to @option{--translate},z see @ref{Merging multiple warpings}. @item -s @itemx --scale (@option{=FLT[,FLT]}) Scale the input image by the given factor. If only one value is given, then both image axes will be scaled with the given value. When two values are given, the first will be used to scale the first axis and the second will be used for the second axis. If you only need to scale one axis, use @option{1} for the axis you don't need to scale. @item -f @itemx --flip (@option{=FLT[,FLT]}) Flip the image around the first, second or both axes. The first value specifies a flip on the first axis and the second on the second axis. The values of the option only matter if they are non-zero. If any of the values are zero, that axis is not flipped. So if you want to flip by the second axis only, use @option{--flip=0,1} (which is equivalent to @option{--flip=0,20} since it only matters if it is non-zero). @item -e @itemx --shear (@option{=FLT[,FLT]}) Apply a shear to the image along the image axes. If only one value is given, then both image axes will be sheared with the given value. When two values are given, the first will be used to shear the first axis and the second will be used for the second axis. If you only need to shear one axis, use @option{0} for the axis you don't need. @item -t @itemx --translate (@option{=FLT[,FLT]}) Apply a translation to the image along the image axes. If only one value is given, then both image axes will be translated with the given value. When two values are given, the first will be used to translate along the first axis and the second will be used for the second axis. If you only need to translate one axis, use @option{0} for the axis you don't need. @item -p @itemx --project (@option{=FLT[,FLT]}) Apply a projection to the image along the image axes. If only one value is given, then the projection will be applied on both image axes with the given value. When two values are given, the first will be used for the first axis and the second will be used for the second axis. If you only need projection along one axis, use @option{0} for the axis you don't need. @item -m @itemx --matrix (@option{=STR}) The warp/transformation matrix. All the elements in this matrix must be separated by any number of space, tab or comma (@key{,}) characters. If you want to use the first two, then be sure to wrap the matrix within double quotation marks (@key{"}) so they are not confused with other arguments on the command-line, see @ref{Options}. This also applies to values in the configuration files, see @ref{Configuration file format}. The transformation matrix can be either 2 by 2 or 3 by 3 array. In the former case (if a 2 by 2 matrix is given), then it is converted to a 3 by 3 matrix with two translation terms added to correct for the FITS definition of position (see @ref{Warping basics}, @ref{Merging multiple warpings}, and the explanations above for more). @cindex NaN The determinant of the matrix has to be non-zero and it must not contain any non-number values (for example infinities or NaNs). The elements of the matrix have to be written row by row. So for the general homography matrix of @ref{Warping basics}, it should be called with @command{--matrix=a,b,c,d,e,f,g,h,1}. @item --nofitscorrect Do not correct for the FITS definition of the pixel center as described in the descriptions above. @item --hstartwcs (@option{=INT}) Specify the first header keyword number (line) that should be used to read the WCS information, see the full explanation in @ref{Invoking astimgcrop}. @item --hendwcs (@option{=INT}) Specify the last header keyword number (line) that should be used to read the WCS information, see the full explanation in @ref{Invoking astimgcrop}. @item -n @itemx --nowcscorrection @cindex WCSLIB @cindex World Coordinate System Do not correct the WCS information of the input image and save it untouched to the output image. By default the WCS (World Coordinate System) information of the input image is going to be corrected in the output image. WCSLIB will save the input WCS information in the @code{PC} matrix@footnote{Greisen E.W., Calabretta M.R. (2002) Representation of world coordinates in FITS. Astronomy and Astrophysics, 395, 1061-1075.}. To correct the WCS, ImageWarp multiplies the @code{PC} matrix with the inverse of the specified transformation matrix. Also the @code{CRPIX} point is going to be changed to its correct place in the output image coordinates. This behavior can be disabled with the @option{--nowcscorrection} option. @cindex Blank pixel @cindex Pixel, blank @item -z @itemx --zerofornoinput Set output pixels which do not correspond to any input to zero. By default they are set to blank pixel values, see @ref{Blank pixels}. @item -b @itemx --maxblankfrac (@option{=FLT}) The maximum fractional area of blank pixels over the output pixel. If an output pixel is covered by blank pixels (see @ref{Blank pixels}) for a larger fraction than the value to this option, the output pixel will be set to a blank pixel its self. When the fraction is lower, the sum of non-blank pixel values over that pixel will be multiplied by the inverse of this fraction to correct for its flux and not cause discontinuities on the edges of blank regions. Note that even with this correction, discontinuities (very low non-blank values touching blank regions in the output image) might arise depending on the transformation and the blank pixels. So if there are blank pixels in the image, a good value to this option has to be found for that particular image and warp. @item -d @itemx --doubletype By default the output image is going to have the same type as the input image. If this option is called, the output will be in double precision floating point format irrespective of the input data type. When dealing with integer input formats, this option can be useful in checking the results. @end table @node SubtractSky, , ImageWarp, Image manipulation @section SubtractSky @cindex Atmosphere @cindex Flat field @cindex Stray light @cindex Bias subtraction Raw astronomical images (and even poorly processed images) don't usually have a uniform `sky' value over their surface prior to processing, see @ref{Sky value} for a complete definition of the sky value. However, a uniform sky value over the image is vital for further processing. For ground based images (particularly at longer wavelengths) this can be due to actual variations in the atmosphere. Another cause might be systematic biases in the instrument or prior processing. For example stray light in the telescope/camera or bad flat-fielding or bias subtraction. The latter is a major issue in space based images where the atmosphere is no longer a problem. @cindex Grid @cindex Mesh @cindex Gradient SubtractSky is a tool to find the sky value and its standard deviation on a grid over the image. The size of the grid will determine how accurately it can account for gradients in the sky value. Such that if the gradient (change of sky value) is too sharp, a smaller grid size has to be chosen. However the results will be most accurate with a larger grid size. @menu * Sky value:: Definition of the sky value. * Tiling an image:: Defining a mesh grid on the image. * Mask image:: How to mask pixels for no analysis. * Invoking astsubtractsky:: Options and arguments to SubtractSky. @end menu @node Sky value, Tiling an image, SubtractSky, SubtractSky @subsection Sky value @cindex Sky value The discussion here is taken from Akhlaghi and Ichikawa (2015)@footnote{See the section on sky in Akhlaghi M., Ichikawa. T. (2015). Astrophysical Journal Supplement Series.}. Let's assume that all instrument defects -- bias, dark and flat -- have been corrected and the brightness (see @ref{Flux Brightness and magnitude}) of a detected object, @mymath{O}, is desired. The sources of flux on pixel @mymath{i}@footnote{For this analysis the dimension of the data (image) is irrelevant. So if the data is an image (2D) with width of @mymath{w} pixels, then a pixel located on column @mymath{x} and row @mymath{y} (where all counting starts from zero and (0, 0) is located on the bottom left corner of the image), would have an index: @mymath{i=x+y\times{}w}.} of the image can be written as follows: @itemize @item Contribution from the target object, (@mymath{O_i}). @item Contribution from other detected objects, (@mymath{D_i}). @item Undetected objects or the fainter undetected regions of bright objects, (@mymath{U_i}). @item @cindex Cosmic rays A cosmic ray, (@mymath{C_i}). @item @cindex Background flux The background flux, which is defined to be the count if none of the others exists on that pixel, (@mymath{B_i}). @end itemize @noindent The total flux in this pixel, @mymath{T_i}, can thus be written as: @dispmath{T_i=B_i+D_i+U_i+C_i+O_i.} @cindex Cosmic ray removal @noindent By definition, @mymath{D_i} is detected and it can be assumed that it is correctly subtracted, so that @mymath{D_i} can be set to zero. There are also methods to detect and remove cosmic rays (for example, van Dokkum (2001)@footnote{van Dokkum, P. G. (2001). Publications of the Astronomical Society of the Pacific. 113, 1420.}) enabling us to set @mymath{C_i=0}. Note that in practice, @mymath{D_i} and @mymath{U_i} are correlated, because they both directly depend on the detection algorithm and its input parameters. Also note that no detection or cosmic ray removal algorithm is perfect. With these limitations in mind, the observed sky value for this pixel (@mymath{S_i}) can be defined as @cindex Sky value @dispmath{S_i=B_i+U_i.} @noindent Therefore, as the detection process (algorithm and input parameters) becomes more accurate, or @mymath{U_i\to0}, the sky value will tend to the background value or @mymath{S_i\to B_i}. Therefore, while @mymath{B_i} is an inherent property of the data (pixel in an image), @mymath{S_i} depends on the detection process. Over a group of pixels, for example in an image or part of an image, this equation translates to the average of undetected pixels. With this definition of sky, the object flux in the data can be calculated with @dispmath{ T_{i}=S_{i}+O_{i} \quad\rightarrow\quad O_{i}=T_{i}-S_{i}.} @noindent @cindex photo-electrons Hence, the more accurately @mymath{S_i} is measured, the more accurately the brightness (sum of pixel values) of the target object can be measured (photometry). Similarly, any under-(over-)estimation in the sky will directly translate to an over(under) estimation of the measured object's brightness. In the fainter outskirts of an object a very small fraction of the photo-electrons in the pixels actually belong to objects. Therefore even a small over estimation of the sky value will result in the loss of a very large portion of most galaxies. Based on the definition above, the sky value is only correctly found when all the detected objects (@mymath{D_i} and @mymath{C_i}) have been removed from the data. @menu * Finding the sky value:: How SubtractSky finds the sky value. * Sky value misconceptions:: Sky value misconceptions and wrong approaches. @end menu @node Finding the sky value, Sky value misconceptions, Sky value, Sky value @subsubsection Finding the sky value @cindex Data @cindex Distribution mode @cindex Distribution mean @cindex Distribution median @cindex Mode of distribution @cindex Mean of distribution @cindex Median of distribution This technique to find the sky value in a distribution was initially proposed in Akhlaghi and Ichikawa 2015@footnote{Akhlaghi M., Ichikawa. T. (2015). Astrophysical Journal Supplement Series.}. Note that through the difference of the mode and median we have actually `detected' data in the distribution. However this detection was only based on the total distribution of the data, not its spatial position in each mesh. So we adhere to the definition of Sky value in @ref{Sky value}. Finding the median is very easy, the main problem is in finding the mode through a robust method. In Appendix C of Akhlaghi and Ichikawa (2015) a new approach to finding the mode in any astronomically relevant distribution is introduced. @cindex Cosmic rays Even when the mode and median are approximately equal, Cosmic rays can significantly bias the calculation of the average. Even if they are very few. However, usually, Cosmic rays have very sharp boundaries and do not fade away into the noise. Therefore, when the histogram of the distribution is plotted, they are clearly separate from the rest of the data. For example see Figure 15 in Akhlaghi and Ichikawa (2015). In such cases, @mymath{\sigma}-clipping is a perfect tool to remove the effect of such objects in the average and standard deviation. See @ref{Sigma clipping} for a complete explanation. So after asserting that the mode and median are approximately equal in a mesh (see @ref{Tiling an image}), convergence-based @mymath{\sigma}-clipping is also applied before getting the final sky value and its standard deviation for a mesh. @node Sky value misconceptions, , Finding the sky value, Sky value @subsubsection Sky value misconceptions As defined in @ref{Sky value}, the sky value is only accurately defined when the detection algorithm is not significantly reliant on the sky value. In particular its detection threshold. However, most signal-based detection tools @footnote{According to Akhlaghi and Ichikawa (2015), signal-based detection is a detection process that relies heavily on assumptions about the to-be-detected objects. This method was the most heavily used technique prior to the introduction of NoiseChisel in that paper.} used the sky value as a reference to define the detection threshold. So these old techniques had to rely on approximations based on other assumptions about the data. A review of those other techniques can be seen in Appendix A of Akhlaghi and Ichikawa (2015)@footnote{Akhlaghi M., Ichikawa. T. (2015). Astrophysical Journal Supplement Series.}. Since they were extensively used in astronomical data analysis for several decades, such approximations have given rise to a lot of misconceptions, ambiguities and disagreements about the sky value and how to measure it. As a summary, the major methods used until now were an approximation of the mode of the image pixel distribution and @mymath{\sigma}-clipping. @itemize @cindex Histogram @cindex Distribution mode @cindex Mode of a distribution @cindex Probability density function @item To find the mode of a distribution those methods would either have to assume (or find) a certain probability density function (PDF) or use the histogram. But the image pixels can have any distribution, and the histogram results are very inaccurate (there is a large dispersion) and depend on bin-widths. @cindex sigma-clipping @item Another approach was to iteratively clip the brightest pixels in the image (which is known as @mymath{\sigma}-clipping, since the reference was found from the image mean and its standard deviation or @mymath{\sigma}). See @ref{Sigma clipping} for a complete explanation. The problem with @mymath{\sigma}-clipping was that real astronomical objects have diffuse and faint wings that penetrate deeply into the noise. So only removing their brightest parts is completely useless in removing the systematic bias an object's fainter parts cause in the sky value. @end itemize As discussed in @ref{Sky value}, the sky value can only be correctly defined as the average of undetected pixels. Therefore all such approaches that try to approximate the sky value prior to detection are ultimately poor approximations. @node Tiling an image, Mask image, Sky value, SubtractSky @subsection Tiling an image @cindex Grid @cindex Tile @cindex Gradient @cindex Mesh grid Some of the programs in Gnuastro will need to divide the pixels in an image into individual tiles or a mesh grid to be able to deal with gradients. In this section we will explain the concept in detail and how the user can check the grid. In the case of SubtractSky, if the image is completely uniform then one sky value will suffice for the whole image. See @ref{Sky value} for the definition of the sky value. Unfortunately though, as discussed in @ref{SubtractSky}, in most images taken with ground or space-based telescopes the sky value is not uniform. So we have to break the image up into small tiles on a mesh grid, assume the sky value is constant over them and find the sky value on those tiles. Meshes are considered to be a square with a side of @option{--meshsize} pixels. The best mesh size is directly related to the gradient on the image. In practice we assume that the gradient is not significant over each mesh. So if there is a strong gradient (for example in long wavelength ground based images) or the image is of a crowded area where there isn't too much blank area, you have to choose a smaller mesh size. A larger mesh will give more pixels and so the scatter in the results will be less. @cindex CCD @cindex Amplifier @cindex Bias current @cindex Subaru Telescope @cindex Hyper Suprime-Cam @cindex Hubble Space Telescope For raw image processing, a simple mesh grid is not sufficient. Raw images are the unprocessed outputs of the camera detectors. Large detectors usually have multiple readout channels each with its own amplifier. For example the Hubble Space Telescope Advanced Camera for Surveys (ACS) has four amplifiers over its full detector area dividing the square field of view to four smaller squares. Ground based image detectors are not exempt, for example each CCD of Subaru Telescope's Hyper Suprime-Cam camera (which has 104 CCDs) has four amplifiers, but they have the same height of the CCD and divide the width by four parts. @cindex Channel The bias current on each amplifier is different, and normally bias subtraction is not accurately done. So even after subtracting the measured bias current, you can usually still identify the boundaries of different amplifiers by eye. See Figure 11(a) in Akhlaghi and Ichikawa (2015) for an example. This results in the final reduced data to have non-uniform amplifier-shaped regions with higher or lower background flux values. Such systematic biases will then propagate to all subsequent measurements we do on the data (for example photometry and subsequent stellar mass and star formation rate measurements in the case of galaxies). Therefore an accurate sky subtraction routine should also be able to account for such biases. To get an accurate result, the mesh boundaries should be located exactly on the amplifier boundaries. Otherwise, some meshes will contain pixels that have been read from two or four different amplifiers. These meshes are going to give very biased results and the amplifier boundary will still be present after sky subtraction. So we define `channel's. A channel is an independent mesh grid that covers one amplifier to ensure that the meshes do not pass the amplifier boundary. They can also be used in subsequent steps as the area used to identify nearby neighbors to interpolate and smooth the final grid, see @ref{Grid interpolation and smoothing}. The number of channels along each axis can be specified by the user at run time through the command-line @option{--nch1} and @option{--nch2} options or in the configuration files, see @ref{Configuration files}. The area of each channel will then be tiled by meshes of the given size and subsequent processing will be done on those meshes. If the image is processed or the detector only has one amplifier, you can set the number of channels in both axes to 1. Unlike the channel size, that has to be an exact multiple of the image size, the mesh size can be any number. If it is not an exact multiple of the image side, the last mesh (rightest, for the first FITS dimension, and highest for the second when viewed in SAO ds9) will have a different size than the rest. If the remainder of the image size divided by mesh size is larger than a certain fraction (value to @option{--lastmeshfrac}) of the mesh size along each axis, a new (smaller) mesh will be put there instead of a larger mesh. This is done to avoid the last mesh becoming too large compared to the other meshes in the grid. Generally, it is best practice to choose the mesh size such that the last mesh is only a few (negligible) pixels wider or thinner than the rest. The final mesh grid can be seen on the image with the @option{--checkmesh} option that is available to all programs which use the mesh grid for localized operations. When this option is called, a multi-extension FITS file with a @file{_mesh.fits} suffix will be created along with the outputs, see @ref{Automatic output}. The first extension will be the input image. For each mesh grid the image produces, there will be a subsequent extension. Each pixel in the grid extensions is labeled to the mesh that it is part of. You can flip through the extensions to check the mesh sizes and locations compared to the input image. @menu * Quantifying signal in a mesh:: Good meshs for gradients. * Grid interpolation and smoothing:: Filling the blank grid elements. * Checking grid values:: Check the values on the grid. * Mesh grid options:: Common options related to the mesh grid. @end menu @node Quantifying signal in a mesh, Grid interpolation and smoothing, Tiling an image, Tiling an image @subsubsection Quantifying signal in a mesh @cindex Noise @cindex Gaussian distribution Noise is characterized with a fixed background value and a certain distribution. For example, for the Gaussian distribution these two are the mean and standard deviation. When we have absolutely no signal and only noise in a data set, the mean, median and mode of the distribution are equal within statistical errors and approximately equal to the background value. For the next paragraph, let's assume that the background is subtracted and is zero. Data always has a positive value and will never become negative, see Figure 1 in Akhlaghi and Ichikawa (2015). Therefore, as data is buried into the noise, the mean, median and mode shift to the positive. The mean is the fastest in this shift. The median is slower since it is defined based on an ordered distribution and so is not affected by a small (less than half) number of outliers. Finally, the mode is the slowest to shift to the positive. Inverting the argument above provides us with the basis of Gnuastro's algorithm to quantify the presence of signal in a mesh. Namely, when the mode and median of a distribution are approximately equal, we can argue that there is no significant signal in that mesh. So we can consider the image to be made of a grid and use this argument to `detect' signal in each grid element. The median is defined to be the value of the 0.5 quantile in the image. So the only necessary parameter is the minimum acceptable quantile (smaller than 0.5) for the mode in a mesh that we deem accurate. See @ref{Mesh grid options} for an explanation of the options used to customize this behavior. Since there is sufficient signal in the mesh to bias the analysis on that mesh, any grid element whose mode quantile is smaller than the minimum acceptable quantile is usually kept with a blank value and no value is given to it. Finally, when all the grid elements have been checked, we can interpolate over all the empty elements and smooth the final result to find the sky value over the full image. See @ref{Grid interpolation and smoothing}. Convolving a data set (that contains signal and noise), creates a positive skewness in it depending on the fraction of data present in the distribution and also the convolution kernel. See Section 3.1.1 in Akhlaghi and Ichikawa (2015) and @ref{Convolution process}. This skewness can be interpreted as an increase in the Signal to noise ratio of the objects buried in the noise. Therefore, to obtain an even better measure of the presence of signal in a mesh, the image can be convolved with a given PSF first. This positive skew will result in more distance between the mode an median thereby enabling a more accurate detection of fainter signal, for example the faint wings of bright stars and galaxies. When convolving over a mesh grid, the pixels in each channel will be treated independently. This can be disabled with the @option{--fullconvolution} option. See @ref{Convolution kernel} for the respective options. @node Grid interpolation and smoothing, Checking grid values, Quantifying signal in a mesh, Tiling an image @subsubsection Grid interpolation and smoothing On some of the grid elements, the desired value will not be found, for example the Sky value in @ref{Finding the sky value}. This can happen for lots of reasons depending on the job that was to be done on a mesh, for example when a large galaxy is present in the image, no Sky value will be found for the grid elements that lie over it. However, the Sky value should be `guessed' over that part of the image. We cannot just ignore those regions! To fill in such blank grid elements, we use interpolation. @cindex Spline interpolation @cindex Linear interpolation @cindex Bicubic interpolation @cindex Interpolation, spline @cindex Interpolation, bicubic @cindex Interpolation, bi-linear Parametric interpolations like bi-linear, bicubic or spline interpolations are not used because they fail terribly on the edges of the image. For example see Figure 16 in Akhlaghi and Ichikawa (2015). They are also prone to cause significant gradients in the image. So to find the interpolated value for each grid element, Gnuastro will look at a certain number of the nearest neighbors. The exact number can be specified through @option{--numnearest}. The median value of those grid elements will be taken as the final value for each mesh. The median is chosen because on the fainter wings of bright objects, the mean can easily become biased. If the number of meshes with a good value is less than the value given to @option{--numnearest}, then the program will abort and notify you. In such cases you can either decrease the value to this option or set less restrictive requirements (for example a smaller @option{--minmodeq}, or larger/smaller meshs) at the expense of less accurate results. @cindex PSF By default the process above will occur on all the grid elements, not just the ones that are blank. This is done to avoid biased results on the faint wings of bright galaxies and stars (the PSF). Because their flux penetrates into the noise very slowly, it might not be possible to completely identify that flux and ignore that mesh. Therefore, if interpolation is only done on blank pixels, such false positives can cause a bias in the vicinity of bright objects, particularly after smoothing in the next step. In order to only interpolate over blank meshs and leave the values of the successful meshs untouched, the @option{--interponlyblank} option can be used. @cindex Average filter Once all the grid elements are filled, the values given to all the meshs should be smoothed. This is because the median was used in the interpolation. The median is robust in the face of outliers, but there might be strong differences from one grid element to the next. By smoothing the grid, the variation between grid element to grid element will be far less. To smooth the mesh values, Gnuastro uses an average filter. An average filter is just a convolution of the mesh grid (spatial convolution with edge correction) by a kernel with all elements having an equal weight, see @ref{Convolution process}. The kernel is a square. The length of the kernel edge can be set in units of meshs through the @option{--smoothwidth} option (which has to be an odd number as with any kernel). If a width of 1 is given for the kernel width, then no smoothing will take place. By default the interpolation and smoothing explained above are done independently on each channel. In some circumstances, it might be preferable to do either one of these two steps on the whole image, independent of the channels. For example when there are gradients over the image and their variation over the image is stronger than the variation caused by the channels. Through the two options @option{--fullinterpolation} and @option{--fullsmooth} you can ask for interpolation or smoothing to use all the meshs in the image, not just those in the same channel of a mesh. Note that it is still very important that no mesh contain pixels from two channels. Since the pixels have been assigned to a mesh prior to these steps (see @ref{Tiling an image}), there is no problem in this regard. Even after smoothing, a simple visual examination of the values given to the pixels in each mesh over the image will give a very `boxy' or pixelated impression. To our eyes it feels that it would be much better if the values could be smoothed in sub-mesh (pixel) scales to obtain a smooth variation. An example is the results of bi-linear and bi-cubic interpolations, see Figure 16 in Akhlaghi and Ichikawa (2015) for several examples. The reasons we are not doing that level of smoothing are two fold: @itemize @item The difference in value between neighboring meshs is not statistically significant. After smoothing, the variation between the neighboring mesh values will be very small. It does visually appear to be a lot when viewing in image viewers like SAO ds9. This is because such viewers use the minimum and maximum range of all the pixel values as a reference to choose the color given to each pixel. However compared to the standard deviation of the noise in the image, the different values of each mesh are completely negligible. Please confirm this for your self on your own datasets to clearly understand. @item Such pixel-based (not mesh-based) interpolation will be very time consuming. Since the difference between the neighboring meshs is statistically negligible, it is simply not worth the time investment. @end itemize @node Checking grid values, Mesh grid options, Grid interpolation and smoothing, Tiling an image @subsubsection Checking grid values Programs that use the mesh grid to calculate some value, also have checking options (that start with @option{--check}). When such options are called, the program will create a specific output file depending on what you want to check. When the operation is done on the meshes, this file shows the values assigned to each mesh grid element. It has three extensions: @enumerate @item The value that was initially calculated for each grid element. If a mesh was not successful in providing a value, a NaN value is stored for that mesh. @item The interpolated values, see @ref{Grid interpolation and smoothing}. @item The smoothed values, see @ref{Grid interpolation and smoothing}. @end enumerate If more than one value is calculated for each mesh (for example the mean and its standard deviation), then each step has that many extensions. By default, these check image outputs have the same size (pixels) as the input image. So all the pixels within a mesh are given the same value. This is useful if you want to later apply these values to the image through another program for example. There is a one to one correspondence between the input image pixels and the grid showing you the mesh values for that pixel. In other situations, the input pixel resolution might not be important for you and you just want to see the relative mesh values over the image. In such cases, you can call the @option{--meshbasedcheck} option so the check image only has one pixel for each mesh. This image will only be as big as the full mesh grid and there will be no world coordinate system. When the input images are really large, this can make a difference in both the processing of the programs and in viewing the images. Another case when only one pixel for each mesh will be useful is when you might want to display the mesh values in a document and you don't want the volume of the document (in bytes) to get too high. For example if the mesh sizes are 30 pixels by 30 pixels, then the mesh grid created through this option will take @mymath{30\times30=900} times less space! You can resize the standard output, but the borders between the meshs will be blurred. The best case is to call that program with this option. @node Mesh grid options, , Checking grid values, Tiling an image @subsubsection Mesh grid options The mesh grid structure defined here (see @ref{Tiling an image}) is used by more than one program. Therefore in order to avoid repetition, all the options to do with the mesh grid (and are shared by all the programs using it) are listed here. Some programs might define multiple meshs over the image (for example in NoiseChisel, there is a large and a small mesh for different operations, see @ref{NoiseChisel}), in such cases, the options for each mesh are designated by an appropriate prefix. For example in NoiseChisel the small and large mesh sizes are specified through the @option{--smeshsize} and @option{--lmeshsize} respectively. Both these options are similar to the @option{--meshsize} option explained below, but for their respective grid. Note that the short option name might also differ. If such options exist in a program, they are listed in the `Invoking ProgramName' section within the list of options. @table @option @item -s @itemx --meshsize (@option{=INT}) The size of each mesh, see @ref{Tiling an image}. If the width of all channels are not an exact multiple of the specified size, then the last mesh on each axis will have a different size to cover the full channel. @item -a @itemx --nch1 (@option{=INT}) The number of channels along the first FITS axis (horizontal when viewed in SAO ds9). If the length of the image is not an exact multiple of this number, then the program will stop. You can use ImageCrop (@ref{ImageCrop}) to trim off or add some pixels (blank pixels if added, see @ref{Blank pixels}) to the image if it is not an exact multiple. @item -b @itemx --nch2 (@option{=INT}) The number of channels along the second FITS axis, (vertical when viewed in SAO ds9). Similar to @option{--nch1}. @item -L @itemx --lastmeshfrac (@option{=FLT}) Fraction of extra area on the last (rightest on the first FITS axis and highest/top on the second) mesh, to define a new (smaller) one. See @ref{Tiling an image}. @item --checkmesh An image with suffix @file{_mesh.fits} will be created for you to check the mesh grid, see @ref{Tiling an image}. The input image will be the first extension, followed by an extension, where each pixel is labeled (number starting from zero) by the ID of the mesh it belongs to. If the program uses multiple mesh grids, the output will have more than two extensions. By flipping through the extensions, you can check the positioning and size of the meshs. @item -d @itemx --mirrordist (@option{=FLT}) The distance beyond the mirror point (in units of the error in the mirror point) to check for finding the mode in each mesh. This is part of the process to quantify the presence of signal in a mesh, see @ref{Quantifying signal in a mesh}. See appendix C in Akhlaghi and Ichikawa (2015) for a complete explanation of the mode-finding algorithm. The value to this option is shown as @mymath{\alpha} in that appendix. @item -Q @itemx --minmodeq (@option{=FLT}) The minimum acceptable quantile for the mode of each mesh. The median is on the 0.5 quantile of the image and as long as we have positive signal (all astronomically relevant observations), the mode will be less than the median. The sky value is only found on meshes where the median and mode are approximately the same, see @ref{Sky value}. @item --interponlyblank Only interpolate the blank pixels. By default, interpolation will happen on all the mesh grids, not just the blank ones. See @ref{Grid interpolation and smoothing}. @item -n @itemx --numnearest (@option{=INT}) The number of nearest grid elements with a successful sky value to use for interpolating over blank mesh elements (those that had a significant contribution of signal), see @ref{Grid interpolation and smoothing}. @item --fullinterpolation Do interpolation irrespective of the channels in the image, see @ref{Grid interpolation and smoothing}. @item -T @itemx --smoothwidth (@option{=INT}) The width of the average filter kernel used to smooth the interpolated image in units of pixels. See @ref{Grid interpolation and smoothing}. If this option is given a value of 1 (one), then no smoothing will be done. @item --fullsmoothing Do smoothing irrespective of the channels in the image, see @ref{Grid interpolation and smoothing}. @item --meshbasedcheck Store the fixed value in each mesh in one check image pixel, see @ref{Checking grid values}. Note that this image has no world coordinate system. @end table @node Mask image, Invoking astsubtractsky, Tiling an image, SubtractSky @subsection Mask image @cindex Mask image All of the programs in Gnuastro that do processing on the input data can also account for masked pixels. Particularly in raw data processing, there are usually a set of pixels in the image that should not be included in any analysis. For example saturated pixels on the centers of bright objects, or the edges of the image which received no data and were only used for bias calculation. The detectors or the very early processing that is done on raw images clearly identifies such cases and usually assigns an integer (or flag or mask value) to those pixels. Pixels that are good for processing usually have a zero value in the mask image. It goes without saying that the two images have to have the same size. Note that if the mask image has blank pixels, then they act like pixels with non-zero values and will be masked (see @ref{Blank pixels}). @cindex Binary mask image values The integer values in the mask images are usually sums of powers of two. Each power of two has a specific meaning and since the sum of two different sets of powers of two are never equal, each mask value identifies a set of different properties for each masked pixels. For some analysis, some masked properties might not be a problem. Therefore a pixel that only has that property should be included. In such cases, you can use bit flags to keep some of the powers of two and remove the rest. The individual Gnuastro programs do not consider these issues. Therefore, if some masked pixels should be included in the analysis, it is best to use another tool to set the appropriate mask pixel values to zero prior to running the analysis program. We are working on such a program as part of Gnuastro. If the data type (@code{BITPIX}) of the input mask image is not an integer type, the programs will print a warning, but continue on with the analysis. This usually happens because of a mistake in specifying the file or the HDU. @cindex NaN The programs that accept a mask image, all share the options below. Any masked pixels will receive a NaN value (or a blank pixel, see @ref{Blank pixels}) in the final output of those programs. In fact, another way to notify any of the Gnuastro programs to not use a certain set of pixels in a data set is to set those pixels equal to appropriate blank pixel value for the type of the image, @ref{Blank pixels}. @table @option @item -M @itemx --mask (@option{=STR}) Mask image file name. If this option is not given and the @option{--mhdu} option has a different value from @option{--hdu}, then the input image name will be used. If a name is specified on the command-line or in any of the configuration files, it will be used. If the program doesn't get any mask file name, it will use all the non-blank (see @ref{Blank pixels}) pixels in the image. Therefore, specifying a mask file name in any of the configuration files is not mandatory. @item -H @itemx --mhdu (@option{=STR}) The mask image header name or number. Similar to the @option{--hdu} option, see @ref{Common options}. Like @option{--mask}, this option does not have to be included in the configuration file or the command-line. However, if it is present on either of them, it will be used. @end table @node Invoking astsubtractsky, , Mask image, SubtractSky @subsection Invoking SubtractSky SubtractSky will find the sky value on a grid in an image and subtract it. The executable name is @file{astsubtractsky} with the following general template: @example $ astsubtractsky [OPTION ...] Image @end example @noindent One line examples: @example $ astsubtractsky image.fits $ astsubtractsky --hdu=0 --mhdu=1 image.fits $ astsubtractsky --nch1=2 --nch2=2 image.fits $ astsubtractsky --mask=maskforimage.fits image.fits @end example @cindex Blank pixel The only required input to SubtractSky is the input data file that currently has to be only a 2D image. But in the future it might be useful to use it for 1D or 3D data too. Any pixels in the image with a blank value will be ignored in the analysis, see @ref{Blank pixels}. Alternatively a mask can be specified which indicates pixels to not be used (see @option{--mask} and @option{--mhdu}). The common options to all Gnuastro programs can be seen in @ref{Common options} and input data formats are explained in @ref{Arguments}. SubtractSky uses a mesh grid to tile the image. This enables it to deal with possible gradients, see @ref{Tiling an image}. The mesh grid options are common to all the programs using it, and are listed in @ref{Mesh grid options}. In order to ignore some pixels during the analysis, you can specify a mask image, see @ref{Mask image} for an explanation and the relevant options. For a more accurate result, a kernel file name can be specified so the image is first convolved, see @ref{Quantifying signal in a mesh}, see @ref{Convolution kernel} for the kernel related options. The @option{--kernel} option is not mandatory and if not specified anywhere prior to running, the original image will be used. Please run SubtractSky with the @option{--help} option to list all the recognized options, irrespective of which part of the book they are fully explained in. @table @option @item -u @itemx --sigclipmultip (@option{=FLT}) The multiple of the standard deviation to clip from the distribution in @mymath{\sigma}-clipping. This is necessary to remove the effect of cosmic rays, see @ref{Sky value} and @ref{Sigma clipping}. @item -t @itemx --sigcliptolerance (@option{=FLT}) The tolerance of sigma clipping. If the fractional change in the standard deviation before and after @mymath{\sigma}-clipping is less than the value given to this option, @mymath{\sigma}-clipping will stop, see @ref{Sigma clipping}. @item --checksky A two extension FITS image ending with @file{_smooth.fits} will be created showing how the interpolated sky value is smoothed. @item --checkskystd In the interpolation and sky checks above, include the sky standard deviation too. By default, only the sky value is shown in all the checks. However with this option, an extension will be added showing how the standard deviation on each mesh is finally found too. @end table @node Image analysis, Modeling and fittings, Image manipulation, Top @chapter Image analysis Astronomical images contain very valuable information, the tools in this section can help in extracting and quantifying that information. For example calculating image statistics, or finding the sky value or detecting objects within an image. @menu * ImageStatistics:: Calculate main image statistics. * NoiseChisel:: Detect objects in an image. * MakeCatalog:: Catalog from input and labeled images. @end menu @node ImageStatistics, NoiseChisel, Image analysis, Image analysis @section ImageStatistics The distribution of pixel values in an image can give us valuable information about the image, for example if it is a positively skewed distribution, we can see that there is significant data in the image. If the distribution is roughly symmetric, we can tell that there is no significant data in the image. On the other hand, in some measurements that we do on the image, we might need to know the certain statistical parameters of the image. For example, if we have run a detection algorithm on an image, and we want to see how accurate it was, one method is to calculate the average of the undetected pixels and see how reasonable it is (if detection is done correctly, the average of undetected pixels should be approximately equal to the background value, see @ref{Sky value}). ImageStatistics is built for precisely such situations. @menu * Histogram and Cumulative Frequency Plot:: Basic definitions. * Sigma clipping:: Definition of @mymath{\sigma}-clipping * Mirror distribution:: Used for finding the mode. * Invoking astimgstat:: Arguments and options to ImageStatistics. @end menu @node Histogram and Cumulative Frequency Plot, Sigma clipping, ImageStatistics, ImageStatistics @subsection Histogram and Cumulative Frequency Plot Histograms and the cumulative frequency plots are both used to study the distribution of data. The histogram is mainly easier to understand for the untrained eye, while the cumulative frequency plot is more accurate, but needs a good level of experience for interpretation. @cindex Histogram @cindex Intervals, histogram @cindex Bin width, histogram @cindex Normalizing histogram @cindex Probability distribution function A histogram shows the number of data points which lie within pre-defined intervals (bins). It is used to get a general view of the distribution and its shape. The width of the bins is one of the most important parameters for a histogram. In the limiting case that the bin-widths tend to zero (and assuming there is data for each bin), then the normalized histogram would show the probability distribution function of the distribution. Normalizing a histogram means to divide the number of data points in each bin by the total number of data. @cindex Cumulative Frequency Plot In the cumulative frequency plot of a distribution, the x axis is the sorted data values and the y axis is the index of each data in the sorted distribution. Unlike a histogram, a cumulative frequency plot does not involve intervals or bins. This makes it less prone to any sort of bias or error that a given bin-width would have on the analysis. When a larger number of the data points have roughly the same value, then the cumulative frequency plot will become steep in that vicinity. This occurs because on the x axis (data values), there is little change while on the y axis the indexes constantly increase. Normalizing a cumulative frequency plot means to divide each index (y axis) by the total number of data points. Unlike the histogram which has a limited number of bins, ideally the cumulative frequency plot should have one point for every data point. Even in small images (for example a @mymath{200\times200}) this will result in an unreasonably larger number of points to plot (40000)! So when the cumulative frequency plot of an image is stored in a text file, it is best to only store its value on a certain number of points (intervals) rather than the whole data. The number of points to use for the final plot can be specified with the @option{--cfpnum} option. Note that the interval's lower value is considered to be part of each interval, but its larger value is not. Formally, an interval between a and b is represented by [a, b). This is true for all the intervals except the last one. The last interval is closed or [a, b]. @node Sigma clipping, Mirror distribution, Histogram and Cumulative Frequency Plot, ImageStatistics @subsection Sigma clipping Let's assume that you have pure noise (centered on zero) with a clear Gaussian distribution, see @ref{Photon counting noise}. Now let's assume you add very bright objects (signal) on the image which have a very sharp boundary. By a sharp boundary, we mean that there is a clear cutoff at the place the objects finish. In other words, at their boundaries, the objects do not fade away into the noise. In such a case, when you plot the histogram (see @ref{Histogram and Cumulative Frequency Plot}) of the distribution, the pixels relating to those objects will be clearly separate from pixels that belong to parts of the image that did not have data. In the cumulative frequency plot, you would observe a long flat region were for a certain range of data (x axis), there is no increase in the index (y axis). @cindex Blurring @cindex Cosmic rays @cindex Aperture blurring @cindex Atmosphere blurring In cases like the above, @mymath{\sigma}-clipping is a very useful tool to remove the effect (bias) of such forms of signal from the distribution. In astronomical applications, cosmic rays (when they collide at a near normal incidence angle) are a very good example of such signals. The tracks they leave behind in the image are perfectly immune to the blurring caused by the atmosphere and the aperture. They are also very energetic and so their borders are usually clearly separated from the surrounding noise. So @mymath{\sigma}-clipping is very useful in removing their effect on the data. See Figure 15 in Akhlaghi and Ichikawa (2015). @mymath{\sigma}-clipping is the very simple iteration below. In each iteration, the range of input data might decrease and so when the data in the image have the conditions above, they will be removed. The criteria to stop the iteration will be discussed below. @enumerate @item Calculate the mean, standard deviation (@mymath{\sigma}) and median (@mymath{m}) of a distribution. @item Remove all points that are smaller or larger than @mymath{m\pm\alpha\sigma}. @end enumerate @noindent The reason the median is used as a reference and not the mean is that the mean is too significantly affected by the presence of signal, while the median is less affected, see @ref{Finding the sky value}. As you can tell from this algorithm, besides the condition above (that the signal have clear high signal to noise boundaries) @mymath{\sigma}-clipping is only useful when the signal does not cover more than half of the full data set. If they do, then the median will lie over the signal and sigma clipping might remove the pixels with no signal. In the literature researchers use either one of two criteria to stop this iteration above: @itemize @item When a certain number of iterations has taken place. @item When the new measured standard deviation is within a certain tolerance level of the old one. The tolerance level is defined by: @dispmath{\sigma_{old}-\sigma_{new} \over \sigma_{new}} The standard deviation is heavily influenced by the presence of outliers. Therefore the fact that it stops changing between two iterations is a sign that we have successfully removed outliers. Note that in each clipping, the dispersion in the distribution is either less or equal. So @mymath{\sigma_{old}\geq\sigma_{new}}. @end itemize @cartouche @noindent Other objects in astronomical data analysis like galaxies and stars are blurred by the atmosphere and the telescope aperture. Galaxies in particular do not appear to have a clear high signal to noise cutoff at all. Therefore @mymath{\sigma}-clipping will not be useful in removing their effect on the data. In astronomy, it is only useful for removing the effect of Cosmic rays. @end cartouche @node Mirror distribution, Invoking astimgstat, Sigma clipping, ImageStatistics @subsection Mirror distribution @cindex Mirror distribution The mirror distribution of a data set was defined in Appendix C of Akhlaghi and Ichikawa (2015). It is best visualized by mentally placing a mirror on the histogram of a distribution at any point within the distribution (which we call the mirror point). Through the @option{--mirrorquant} in ImageStatistics, you can check the mirror of a distribution when the mirror is placed on any given quantile. The mirror distribution is plotted along with the input distribution both as histograms and cumulative frequency plots, see @ref{Histogram and Cumulative Frequency Plot}. Unlike the rest of the histograms and cumulative frequency plots in ImageStatistics, the text files created with the @option{--mirrorquant} and @option{--checkmode} will contain 3 columns. The first is the horizontal axis similar to all other histograms and cumulative frequency plots. The second column shows the respective value for the actual data distribution and the third shows the value for the mirror distribution. @cindex Python The value for each bin of both histogram is divided by the maximum of both. For the cumulative frequency plot, the value in each bin is divided by the maximum number of elements. So one of the cumulative frequency plots reaches the maximum vertical axis of 1. The outputs will have the @file{_mirrorhist.txt} and @file{_mirrorcfp.txt} suffixes respectively. You can use a simple Python script like the one below to display the histograms and cumulative frequency plots in one plot: @example #! /usr/bin/env python3 # Import the necessary modules: import sys import numpy as np import matplotlib.pyplot as plt # Load the two files: a=np.loadtxt(sys.argv[1]+"_mirrorhist.txt") b=np.loadtxt(sys.argv[1]+"_mirrorcfp.txt") # Calculate the bin width: w=a[1,0]-a[0,0] # Plot the two histograms and cumulative frequency plots: plt.bar(a[:,0], a[:,1], width=w, color="blue", linewidth=0, alpha=0.6) plt.bar(a[:,0], a[:,2], width=w, color="green", linewidth=0, alpha=0.4) plt.plot(b[:,0], b[:,1], linewidth=2, color="blue") plt.plot(b[:,0], b[:,2], linewidth=2, color="green") # Write the axis labels: plt.ylim([0,np.amax(a[:,1])]) plt.xlim([np.amin(a[:,0]),np.amax(a[:,0])]) # Save the output to any name from the command-line: plt.savefig(sys.argv[1]+"_plot.pdf") @end example @cindex PNG @cindex Matplotlib @noindent The output format can be anything that Python's Matplotlib recognizes (for example png or jpg are also acceptable). So, if your input data file name was @file{input.fits}, and you want to see how its mirror distribution would look like if the mirror was placed at the 0.8 quantile (or the value which is above 80 percent of your data) you can run the following sequence of commands to see the combined cumulative frequency plot and histogram together in one PDF file. Let's assume you have put the Python script above into the file @file{mirrorplot.py}. The second command makes the Python script an executable file. @example $ ls input.fits mirrorplot.py $ chmod +x mirrorplot.py $ astimgstat input.fits --nohist --nocfp --mirrorquant=0.8 $ ls input.fits input_mirrorcfp.txt input_mirrorhist.txt mirrorplot.py $ ./mirrorplot.py input @end example By default, the range of the mirror distribution is set to the 0.01 quantile of the image to 2 times the distance of the mode to that point. This is done so that the mode (which will have a value of zero in this plot) is positioned exactly on 1/3rd point of the x axis plot. The number of bins is the same value as the @option{--histnumbins} option. Alternatively, through the option @option{--histrangeformirror}, the histogram properties set with the @option{--histmin} and @option{--histmax} can be used. In these mirror plots, the mirror value is going to have the value of zero and one of the bins is going to start at zero (if @option{--histrangeformirror} is called, the given ranges will also shift accordingly). @node Invoking astimgstat, , Mirror distribution, ImageStatistics @subsection Invoking ImageStatistics ImageStatistics will print the major statistical measures of an image's pixel value distribution. The executable name is @file{astimgstat} with the following general template @example $ astimgstat [OPTION ...] InputImage.fits @end example @noindent One line examples: @example $ astimgstat input.fits $ astimgstat animage.fits --ignoremin --nohist $ astimgstat anotherimage.fits --mask=detectionlabels.fits --mhdu=1 @end example @noindent If ImageStatistics is to do any data processing, an input image should be provided with the recognized extensions as input data, see @ref{Arguments}. See @ref{Common options} for the list of options that are shared by all programs. All the main statistical operations have their specific set of options. If a string is given to the @option{--output} option, it is used as the base name for the generated files. Without this option, the input image name is used as the name-base. Some of the options are necessary and if they are not included in the configuration file, ImageStatistics will not run, see @ref{Configuration files}. However, for some others this is not so: @option{--histmin}, @option{--histmax}, @option{--histquant}, @option{--cfpmin}, @option{--cfpmax}, @option{--cfpquant}. These are options to do with the range of values in the histogram and cumulative frequency plots. If no value is given for these options when ImageStatistics is about to start processing the data, then the full data range will be used. Such that the minimum image value will be set for the minimums and the maximum image value will be used for the maximum. The Mask name and HDU are also not mandatory in the configuration file. @cindex ASCII plot By default, in verbose mode @footnote{If the @option{-q} option is not called then all programs will operate in verbose mode, see @ref{Common options}.}, along with a short summary of the basic data statistics, a simple ASCII histogram will also be printed. This can be useful for a very quick and general view of the distribution. An example verbose output of ImageStatistics on one of the @command{$ make check} outputs can be seen below: @example $ astimgstat ./tests/convolve_spatial_warped_noised.fits \ --histquant=0.05 ImageStatistics started on AAA BBB CC DD:EE:FF GGGG - Input read: ./tests/convolve_spatial_warped_noised.fits (hdu: 0) -- Number of points 10000 -- Minimum -38.2066 -- Maximum 1268.72 -- Sum 154927 -- Mean 15.4927 -- Standard deviation 60.5407 -- Median 4.82691 -- Mode (quantile, value) 0.4335, 2.90301 -- Mode symmetricity and its cutoff value 0.5909, 17.2507 -- ASCII histogram in the range: -13.912957 -- 65.058487: | * * | ******** | ********* ** | ************** | ****************** | ******************** | *********************** |*************************** |****************************** |***************************************** |************************************************************ |------------------------------------------------------------ - Sigma clipping results (Median, Mean, STD, Number): - 4.00 times sigma by convergence (tolerance: 0.2000): 1: 4.826907, 15.492665, 60.540707, 10000 2: 4.665353, 10.117773, 27.793823, 9881 3: 4.433090, 7.458610, 18.510950, 9715 4: 4.216213, 6.176818, 15.231371, 9575 5: 4.088199, 5.679162, 14.183748, 9502 - 4.00 sigma-clipping 5 times: 1: 4.826907, 15.492665, 60.540707, 10000 2: 4.665353, 10.117773, 27.793823, 9881 3: 4.433090, 7.458610, 18.510950, 9715 4: 4.216213, 6.176818, 15.231371, 9575 5: 4.088199, 5.679162, 14.183748, 9502 ImageStatistics finished in: 0.006964 (seconds) @end example @table @option @item -M @itemx --mask (@option{=STR}) The file name of a mask image. If this option is not given on the command-line or in the configuration files and @option{--mhdu} is not given or is identical to @option{--hdu}, then no mask image will be used. @item -H @itemx --mhdu (@option{=STR}) The header name of the mask extension. @item -r @itemx --ignoremin Ignore all data elements that have a value equal to the minimum value in the image. In practice this is like masking those pixels, their values will not be used. @item -l @itemx --lowerbin Set the first column of the histogram and cumulative frequency plots to the lower interval boundary. By default (without calling this option), the central interval value is used. @item --onebinvalue (@option{=FLT}) Make sure that one bin starts with the value to this option. In practice, this will shift the bins used to find the histogram and cumulative frequency plot such that one bin's lower interval becomes this value. For example when the histogram range includes negative values, but the data doesn't. If zero is somewhere between one bin, then the viewers of the plot(s) will think negative data is also present. By setting @option{--onebinvalue=0}, you can make sure that the viewers of the histogram will not be confused. @cindex NaN Note that by default, the first row of the histogram and cumulative frequency plot show the central values of each bin. So in the example above you will not see the 0.000. To see it, add the @option{--lowerbin} option to show the lower value of each bin. If you don't care about the bin positions within the specified range you can set the value to this option to a Not-a-Number (NaN) value on the command-line (@option{--onebinvalue=nan}) or in the configuration files with a @code{nan} following the option name. If the value is not within the specified bin range, it will be ignored. @item --noasciihist Do not show an ASCII plot on the command-line. @item --mirrorquant (@option{=FLT}) quantile to put the mirror. A value between 0 and 1. See @ref{Mirror distribution} for a complete explanation. Outputs two files with suffixes @file{_mirrorhist.txt} and @file{_mirrorcfp.txt}. @item --checkmode The mode of the data is found by comparing the input data distribution with its mirror distribution. If this option is called, the mirror distribution's histogram and cumulative frequency plots will be saved in to plain text files ending with @file{_modehist.txt} and @file{_modecfp.txt}. See the explanation for @ref{Mirror distribution} for more details about these two files and how you can easily plot the outputs. This option only works when when ImageStatistics is in verbose mode. Since otherwise the mode is not calculated. To draw the plots you can use the script in @ref{Mirror distribution}. Just change the appended suffixes in the two calls to @code{np.loadtxt} in the Python script. @item --histrangeformirror Use @option{--histmin} and @option{--histmax} for the range of the mirror distributions (which are produced with the @option{--mirrorquant} and @option{--checkmode} options). @end table @noindent @strong{Histogram:} The stored histogram is stored in a text file ending with @file{_hist.txt}. @table @option @item --nohist Do not calculate or save the histogram. @item --normhist Make a normalized histogram, see @ref{Histogram and Cumulative Frequency Plot}. @item --maxhistone Divide all histogram bins by the number in the bin with the most data points. This is very useful if you want to plot the histogram along with a normalized cumulative frequency plot in one plot. Note that if the histogram numbers are important in showing along with the cumulative frequency plot, you can use @option{--maxcfpeqmaxhist}, see below. @item -n @itemx --histnumbins (@option{=INT}) The number of bins in the histogram. Note that in practice, this is also equivalent to the number of rows in the output text file. @item -i @itemx --histmin (@option{=FLT}) The minimum value to use in the histogram. If @option{--histquant} is given, then any value given @option{--histmin} or @option{--histmax} is ignored. @item -x @itemx --histmax (@option{=FLT}) The maximum value to use in the histogram. Similar to @option{--histmin}. @item -Q @itemx --histquant (@option{=FLT}) Set the range of the histogram based on the image quantile. So @option{--histquant=0.05} is given, all the data from the 0.05 quantile to 0.95 quantile will be used in the histogram. This is useful when there is a small number of outliers in the image. Note that if this option is given, any (possible) value given to @option{--histmin} or @option{--histmax} are ignored. @end table @noindent @strong{Cumulative Frequency Plot:} The cumulative frequency plot will be stored in a text file ending with @file{_cfp.txt}. To be more realistic, the average of the indexs in each interval is used as the second column, see @ref{Histogram and Cumulative Frequency Plot}. @table @option @item --nocfp Do not calculate or store the cumulative frequency plot. @item --normcfp Normalize the cumulative frequency plot, see @ref{Histogram and Cumulative Frequency Plot}. @item --maxcfpeqmaxhist Set the maximum cumulative frequency plot value to the maximum value in the histogram (if it is to be created). This is a useful in plotting the histogram and cumulative frequency plots together when the histogram numbers are important. @item --cfpsimhist Set the range of the cumulative frequency plot and the number of points to store to the same range as the histogram. If the two are to be plotted together, this is very useful, since the first axis (column) of the two will become identical. @item -p @itemx --cfpnum (@option{=INT}) The number of points to store the cumulative frequency plot. They will be evenly distributed between the range of pixel values. @item -a @itemx --cfpmin (@option{=FLT}) The minimum value to use for the cumulative pixel value range. If @option{--cfpquant} is given, then any value given @option{--cfpmin} or @option{--cfpmax} is ignored. @item -n @itemx --cfpmax (@option{=FLT}) The maximum value to use for the cumulative pixel value range. Similar to @option{--cfpmin}. @item -U @itemx --cfpquant (@option{=FLT}) Similar to @option{--histquant} but for the cumulative frequency plot. @end table @noindent @strong{@mymath{\sigma}-clipping:} The result of each iteration of @mymath{\sigma}-clipping will be printed in the terminal for both types of sigma clipping: A certain number of times and convergence of the standard deviation. @table @option @item --nosigclip If this option is called, no @mymath{\sigma}-clipping will take place. @item -u @itemx --sigclipmultip (@option{=FLT}) The multiple of the standard deviation above which to clip. This value is demonstrated by @mymath{\alpha} in @ref{Sigma clipping}. @item -t @itemx --sigcliptolerance (@option{=FLT}) If the fractional difference of the standard deviation becomes less than this value, then @mymath{\sigma}-clipping will halt, see @ref{Sigma clipping}. @item -g @itemx --sigclipnum (@option{=INT}) The number of iterations for the case where the @mymath{\sigma}-clipping iteration stops after a certain number of runs. @end table @node NoiseChisel, MakeCatalog, ImageStatistics, Image analysis @section NoiseChisel Once raw data have gone through the initial reduction process (through the programs in @ref{Image manipulation}). We are ready to derive scientific results out of them. Unfortunately in most cases, the scientifically interesting targets are deeply drowned in a sea of noise. NoiseChisel is Gnuastro's tool to detect signal in noise. In fact, NoiseChisel was the motivation behind creating Gnuastro and has a journal article devoted to its techniques: @url{http://arxiv.org/abs/1505.01664, arXiv:1505.01664}, published in 2015 by the Astrophysical Journal Supplement Series 220. Following the explanations for the options in @ref{NoiseChisel options} should provide a relatively good idea of how NoiseChisel works, but it is recommended to see the paper since it does a very thorough job at explaining the concepts and methods of NoiseChisel with abundant demonstrations for each step. However, the paper cannot undergo any further updates, but NoiseChisel will evolve: better algorithms or steps will be found, thus options will be added or removed. So this section is the definitive guide. Please follow the @file{NEWS} file with each release for such updates. @cindex Detection Detection is the process of separating signal from noise. In other words, after detection is complete, one set of data elements (pixels in an image) will be distinguished as signal and another set of the data elements will be noise. Segmentation is the process of labeling the detected pixels into possibly multiple components (objects). For example when two galaxies lie sufficiently close to each other to be detected as one object. @cindex Noise-based detection NoiseChisel was the first software to make use of a noise-based concept to detection and segmentation. In this method, instead of emphasizing on the signal and trying to guess the properties of the to-be-detected targets prior to detection (for example assuming that it is an ellipse), the emphasis is put on the noise in the image and it imposes statistically negligible requirements on the signal. The name of NoiseChisel is derived from the first thing it does after thresholding the image: to erode it. In mathematical morphology, erosion on pixels can be pictured as carving off boundary pixels. So what NoiseChisel does is similar to what a wood chisel or stone chisel do. It is just not a hardware but software. @menu * Invoking astnoisechisel:: Options and arguments for NoiseChisel. @end menu @node Invoking astnoisechisel, , NoiseChisel, NoiseChisel @subsection Invoking NoiseChisel NoiseChisel will detect signal in noise. The executable name is @file{astnoisechisel} with the following general template @example $ astnoisechisel [OPTION ...] InputImage.fits @end example @noindent One line examples: @example $ astnoisechisel input.fits $ astnoisechisel --nch1=4 --lmesh=256 input.fits $ astnoisechisel field.fits --mask=badpixels.fits --mhdu=1 @end example @cindex Gaussian @noindent If NoiseChisel is to do processing, an input image should be provided with the recognized extensions as input data, see @ref{Arguments}. The options that are shared by all Gnuastro programs can be seen in @ref{Common options}. In order to ignore some pixels during the analysis, you can specify a mask image, see @ref{Mask image} for an explanation and the relevant options. A masked pixel is completely ignored. A convolution kernel can also be optionally given. If a value (file name) is given to @option{--kernel} on the command-line or in a configuration file (see @ref{Configuration files}), then that file will be used to convolve the image prior to thresholding. Otherwise a default kernel will be used. The default kernel is a 2D Gaussian with a FWHM of 2 pixels truncated at 5 times the FWHM. See Section 3.1.1 of Akhlaghi and Ichikawa (2015) to learn why this particular kernel was chosen as default. See @ref{Convolution kernel} for kernel related options. NoiseChisel uses a mesh grid to tile the image. This enables it to deal with possible gradients, see @ref{Tiling an image}. The mesh grid options are common to all the programs using it, and are listed in @ref{Mesh grid options}. In particular, NoiseChisel uses two mesh grids: a large and a small one. The sizes of the meshs in each grid can be specified with the following two options (the @option{--meshsize} option is not recognized by NoiseChisel). The rest of the options explained in @ref{Mesh grid options} apply to both grids. @table @option @item -s @itemx --smeshsize Similar to @option{--meshsize} in @ref{Mesh grid options}, but for the smaller mesh grid, which is most dependent on the gradients in the image. @item -l @itemx --lmeshsize Similar to @option{--meshsize} in @ref{Mesh grid options}, but for the larger mesh grid, used for detection and segmentation Signal to noise ratio analysis. @end table @noindent Please run NoiseChisel with the @option{--help} option to list all the recognized options with a short explanation, irrespective of which part of the Gnuastro book they are fully explained in, see @ref{Getting help}. @menu * NoiseChisel options:: The options specific to NoiseChisel. * NoiseChisel output:: NoiseChisel's output. Why no catalog? @end menu @node NoiseChisel options, NoiseChisel output, Invoking astnoisechisel, Invoking astnoisechisel @subsubsection NoiseChisel options The options particular to NoiseChisel are listed below. They are classified by context and also sorted in the same order that the operations are done on the image. See Akhlaghi and Ichikawa (2015) for a very complete, detailed and illustrated explanation of each step. Reading through the option explanations should be enough to obtain a general idea of how NoiseChisel works. Before the procedures explained by these options begin, the image is convolved with a kernel. The first group of options listed below are those that apply to both the detection and the segmentation processes. @table @option @item -E @itemx --skysubtracted If this option is called, it is assumed that the image has already been sky subtracted once. Knowing if the sky has already been subtracted once or not is very important in estimating the Signal to noise ratio of the detections and clumps. In short an extra @mymath{\sigma_{sky}^2} must be added in the error (noise or denominator in the Signal to noise ratio) for every flux value that is present in the calculation. This can be interpreted as the error in measuring that sky value when it was subtracted by any other program. See Section 3.3 in Akhlaghi and Ichikawa (2015) for a complete explanation. @item -B @itemx --minbfrac (@option{=FLT}) Minimum fraction (value between 0 and 1) of blank (undetected) area in a mesh for it to be considered in measuring the following properties. @itemize @item Measuring the Signal to noise ratio of false detections during the false detection removal. @item Measuring the sky value (average of undetected pixels). Both before the removal of false detections and after it. @item Clump Signal to noise ratio in the blank regions. @end itemize Because of the PSF, astronomical objects, other than cosmic rays, never have a clear cutoff and commonly sink into the noise very slowly. Even below the very low thresholds used by NoiseChisel. So when a large fraction of the area of one mesh is covered by detections, it is very probable that their faint wings are present in the undetected regions. Therefore, to get an accurate measurement of the above parameters over the full mesh grid, meshs that harbor too many detected regions should be excluded. @item -F @itemx --minnumfalse (@option{=INT}) The minimum number of `psudo-detections' (in identifying false detections) or clumps (in identifying false clumps) in each large mesh grid. If their number is less than this value, this mesh will be left blank and filled during mesh interpolation, see @ref{Grid interpolation and smoothing}. The Signal to noise ratio of false detections and clumps in each mesh is found using the quantile of the Signal to noise ratio distribution of the psudo-detections and clumps over the undetected pixels in each mesh. If the number of Signal to noise ratio measurements in each mesh is not enough, the quantile will not be accurate. For example if you set @option{--detquant=0.99} (or the top 1 percent), then it is best to have at least 100 Signal to noise ratio measurements. @end table @noindent Detection is the process of separating the pixels in the image into two groups: 1) Signal and 2) Noise. Through the parameters below, you can customize the detection process in NoiseChisel. @table @option @item -t @itemx --qthresh (@option{=FLT}) The quantile threshold to apply to the convolved image. The detection process begins with applying a quantile threshold to each of the small mesh grid elements, see @ref{Tiling an image}. The quantile is only calculated for those meshs that don't have any significant signal within them, see @ref{Quantifying signal in a mesh}. @cindex Quantile @cindex Binary image @cindex Foreground pixels @cindex Background pixels The quantile value is a floating point value between 0 and 1. Assume that we have sorted the @mymath{N} data elements of a distribution (the pixels in each mesh on the convolved image). The quantile (@mymath{q}) of this distribution is the value of the element with an index of (the nearest integer to) @mymath{q\times{N}} in the sorted data set. After thresholding is complete, we will have a binary (two valued) image. The pixels above the threshold are known as foreground pixels (have a value of 1) while those which lie below the threshold are known as background (have a value of 0). @cindex NaN @item --checkthreshold Check the quantile threshold values on the mesh grid. A file suffixed with @file{_thresh.fits} will be created, see @ref{Checking grid values}. @item -e @itemx --erode @cindex Erosion (@option{=INT}) The number of erosions to apply to the binary thresholded image. Erosion is simply the process of flipping (from 1 to 0) any of the foreground pixels that neighbor a background pixel. In a 2D image, there are two kinds of neighbors, 4-connected and 8-connected neighbors. You can specify which type of neighbors should be used for erosion with the @option{--erodengb} option, see below. Erosion has the effect of shrinking the foreground pixels. To put it another way, it expands the holes. This is a founding principle in NoiseChisel: it exploits the fact that with very low thresholds, the holes in the very low surface brightness regions of an image will be smaller than regions that have no signal. Therefore by expanding those holes, we are able to separate the regions harboring signal. @item --erodengb (@option{=4or8}) The type of neighborhood (structuring element) used in erosion, see @option{--erode} for an explanation on erosion. In 4-connectivity, the neighbors of a pixel are defined as the four pixels on the top, bottom, right and left of a pixel that share an edge with it. The 8-connected neighbors on the other hand include the 4-connected neighbors along with the other 4 pixels that share a corner with this pixel. See Figure 6 (a) and (b) in Akhlaghi and Ichikawa (2015) for a demonstration. @item --noerodequant Pure erosion is going to carve off sharp and small objects completely out of the detected regions. This option can be used to avoid missing such sharp and small objects (which have significant pixels, but not over a large area). All pixels with a value larger than the significance level specified by this option will not be eroded during the erosion step above. However, they will undergo the erosion and dilation of the opening step below. Like the @option{--qthresh} option, the significance level is determined using the quantile (a value between 0 and 1). Just as a reminder, in the normal distribution, @mymath{1\sigma}, @mymath{1.5\sigma}, and @mymath{2\sigma} are approximately on the 0.84, 0.93, and 0.98 quantiles. @item -p @itemx --opening (@option{=INT}) Depth of opening to be applied to the eroded binary image. Opening is a composite operation. When opening a binary image with a depth of @mymath{n}, @mymath{n} erosions (explained in @option{--erode}) are followed by @mymath{n} dilations. Simply put, dilation is the inverse of erosion. When dilating an image any background pixel is flipped (from 0 to 1) to become a foreground pixel. Dilation has the effect of fattening the foreground. Note that in NoiseChisel, the erosion which is part of opening is independent of the initial erosion that is done on the thresholded image (explained in @option{--erode}). The structuring element for the opening can be specified with the @option{--openingngb} option. Opening has the effect of removing the thin foreground connections (mostly noise) between separate foreground `islands' (detections) thereby completely isolating them. Once opening is complete, we have @emph{initial} detections. @item --openingngb (@option{=4or8}) The structuring element used for opening, see @option{--erodengb} for more information about a structuring element. @item -u @itemx --sigclumpmultip (@option{=FLT}) The multiple of the standard deviation during @mymath{\sigma}-clipping. NoiseChisel uses @mymath{\sigma}-clipping to remove the effect of cosmic rays when calculating the average and standard deviation of the undetected regions. Since cosmic rays have sharp boundaries and are usually small, the erosion and opening might put them within the undetected pixels. Although they might cover a very small number of pixels, they usually have very large flux values which can easily bias the average and standard deviation measured on a mesh. Their effect can easily be removed by @mymath{\sigma}-clipping, see @ref{Sigma clipping}. NoiseChisel uses the convergence of the value of the standard deviation as the criteria to stop the @mymath{\sigma}-clipping iteration. @item -r @itemx --sigcliptolerance (@option{=FLT}) The tolerance level to stop @mymath{\sigma}-clipping. The iteration is stopped when @mymath{(\sigma_{old}-\sigma_{new})/\sigma_{new}} becomes smaller than the value given to this option. Note that @mymath{\sigma_{old}} will always be larger than @mymath{\sigma_{new}}. Only statistical scatter (error) can cause it to be smaller, in which case they can be considered to be approximately equal. @item --checkdetectionsky Check the initial approximation of the sky value and its standard deviation in a FITS file ending with @file{_detsky.fits}. See @ref{Checking grid values} for more information. If @option{--meshbasedcheck} is not called, then the first extension will be the the binary image with initial detections labeled one and background labeled zero. The mesh values will be in the subsequent extensions. @item -R @itemx --dthresh (@option{=FLT}) The detection threshold: a multiple of the initial sky standard deviation added with the initial sky approximation. This flux threshold is applied to the initially undetected regions on the unconvolved image. The background pixels that are completely engulfed in a 4-connected foreground region are converted to background (holes are filled) and one opening (depth of 1) is applied over both the initially detected and undetected regions. The Signal to noise ratio of the resulting `psudo-detections' are used to identify true vs. false detections. See Section 3.1.5 and Figure 7 in Akhlaghi and Ichikawa (2015) for a very complete explanation. @item -i @itemx --detsnminarea (@option{=INT}) The minimum area to calculate the Signal to noise ratio on the psudo-detections of both the initially detected and undetected regions. When the area in a psudo-detection is too small, the Signal to noise ratio measurements will not be accurate and their distribution will be heavily skewed to the positive. So it is best to ignore any psudo-detection that is smaller than this area. Use @option{--detsnhistnbins} to check if this value is reasonable or not. @item --detsnhistnbins (@option{=INT}) If not equal to zero, a histogram of the Signal to noise ratios of the psudo-detections will be stored in a text file ending with @file{_detsn.txt}. The number of bins in this histogram is specified by the value given to this option. This is good for inspecting the best possible value to @option{--detsnminarea}. An empirical way to estimate the best @option{--detsnminarea} value for your data set is that the histogram have a sharp drop towards the higher S/Ns. In other words, when there is a prominent peak in the histogram and the last few bins have less than 10 (an arbitrary number, meaning very few!) pseudo-detections. When the minimum area is too large or too small, the slope of the histogram in the higher S/N bins will not be to sharp with the very high S/N bins having a large number of objects and the peak being less significant. A good minimum area will result in the last bins having very few pseudo-detections. @item -c @itemx --detquant (@option{=FLT}) The quantile of the Signal to noise ratio distribution of the psudo-detections in each mesh to use for filling the large mesh grid. Note that this is only calculated for the large mesh grids that satisfy the minimum fraction of undetected pixels (value of @option{--minbfrac}) and minimum number of psudo-detections (value of @option{--minnumfalse}). @item -I @itemx --dilate (@option{=INT}) Number of times to dilate the final true detections. See the explanations in @option{--opening} for more information on dilation. The structuring element for this final dilation is fixed to an 8-connected neighborhood. This is because astronomical objects, except cosmic rays, never have a clear cutoff, so all the 8-pixels connected to the border pixels of a detection might harbor data. @item --checkdetection Every step of the detection process will be added as an extension to a file with the suffix @file{_det.fits}. Going through each would just be a repeat of the explanations above and also of those in Akhlaghi and Ichikawa (2015). The extension label should be sufficient to recognize which step you are observing. Viewing all the steps can be the best guide in choosing the best set of parameters. Note that calling this function will significantly slow NoiseChisel. Normally the detection steps are done in parallel, but to show you each step individually, the parallel processing has to be halted and restarted multiple times. Below are some notes that might be useful in interpreting certain steps, beyond the paper. @itemize @item Going from the first ``Labeled'' extension (for the background pseudo-detections, which shows the labeled pseudo-detections) to the next extension (``For S/N''), with a relatively low @option{--dthresh} value, you will notice that a lot of the large area pseudo-detections are removed and not used in calculating the S/N threshold. The main reason for this is that they overlap with possible detections. You can check by going to the next extension and seeing how there are detections there. The filled holes have been covering initial detections. If you have many such cases, it might be a good sign that your @option{--dthresh} value is too low. @end itemize @item --checksky Check the final sky and its standard deviation values on the mesh grid. Similar to @option{--checkdetectionsky}. @item --checkmaskdet Mask (set to NaN) the undetected pixels in one extension and the detected pixels in the next extension of a file ending with @file{_maskdet.fits}. @end table @noindent Segmentation is the process of possibly breaking up a detection into multiple objects and clumps. In deep surveys segmentation becomes particularly important since galaxies might fall along the same line of sight or they might be merging. It is thus very important to be able separate the pixels within a detection if it is necessary. After segmentation, such a detected region will get different labels. In NoiseChisel, segmentation is done by first finding the `true' clumps over a detection and then expanding those clumps to a certain flux limit. True clumps are found in a process very similar to the true detections explained above, see Akhlaghi and Ichikawa (2015) for more information. If the connections between the grown clumps are weaker than a given threshold, the grown clumps are considered to be separate objects. Otherwise, the are considered to be part of the same object. @table @option @item --detectonly If this option is called, no segmentation will be done. The object labels extension in the output will simply be the detection (connected components) labels and the clumps image will be blank (see @ref{NoiseChisel output}). This option can result in faster processing when only the noise properties of the image are desired for a catalog using another image's labels. A common case is when you want to measure colors or SEDs in several images. Let's say you have images in two colors: A and B. For simplicity also assume that they are exactly on the same position in the sky with the same pixel scale. You choose to set A as a reference, so you run the full NoiseChisel on A. Then you run NoiseChisel on B with this option since you only need the noise properties of B (for the signal to noise column in its catalog). You can then run MakeCatalog on A normally, see @ref{MakeCatalog}. To run MakeCatalog on B, you simply set the object and clump labels images to those that NoiseChisel produced for A, see @ref{Invoking astmkcatalog}. @item -m @itemx --segsnminarea (@option{=INT}) The minimum area which a clump in the undetected regions should have in order to be considered in the clump Signal to noise ratio measurement. If this size is set to a small value, the Signal to noise ratio of false clumps will not be accurately found. Note that this has to be larger than the value to @option{--detsnminarea}. Because the clumps are found on the convolved (smoothed) image while the psudo-detections are found on the input image. Use @option{--clumpsnhistnbins} to check if this value is reasonable or not. @item --clumpsnhistnbins (@option{=INT}) Similar to @option{--detsnhistnbins} (see there for more explanations), but for the distribution of the S/N of clumps over the undetected regions. The relevant parameter to check here is be @option{--segsnminarea}. @item -g @itemx --segquant (@option{=FLT}) The quantile of the noise clump Signal to noise ratio distribution. This value is used to identify true clumps over the detected regions. @item -v @itemx --keepmaxnearriver Keep a clump whose maximum flux is 8-connected to a river pixel. By default such clumps over detections are considered to be noise and are removed irrespective of their brightness (see @ref{Flux Brightness and magnitude}). Over large profiles, that sink into the noise very slowly, noise can cause part of the profile (which was flat without noise) to become a very large and with a very high Signal to noise ratio. In such cases, the pixel with the maximum flux in the clump will be immediately touching a river pixel. @item -G @itemx --gthresh (@option{=FLT}) Threshold (multiple of the sky standard deviation added with the sky) to stop growing true clumps. Once true clumps are found, they are set as the basis to segment the detected region. They are grown until the threshold specified by this option. @item --grownclumps In the output (see @ref{NoiseChisel output}) store the grown clumps (or full detected region if only one clump was present in that detection). By default the original clumps are stored as the third extension of the output, if this option is called, it is replaced with the grown clump labels. @item -y @itemx --minriverlength (@option{=INT}) The minimum length of a river between two grown clumps for it to be considered in Signal to noise ratio estimations. Similar to @option{--segsnminarea} and @option{--detsnminarea}, if the length of the river is too short, the Signal to noise ratio can be noisy and unreliable. Any existing rivers shorter than this length will be considered as non-existent, independent of their Signal to noise ratio. Since the clumps are grown on the input image, this value should best be similar to the value of @option{--detsnminarea}. Recall that the clumps were defined on the convolved image so @option{--segsnminarea} was larger than @option{--detsnminarea}. @item -O @itemx --objbordersn (@option{=FLT}) The maximum Signal to noise ratio of the rivers between two grown clumps in order to consider them as separate `objects'. If the Signal to noise ratio of the river between two grown clumps is larger than this value, they are defined to be part of one `object'. Note that the physical reality of these `objects' can never be established with one image, or even multiple images from one broad-band filter. Any method we devise to define `object's over a detected region is ultimately subjective. Two very distant galaxies or satellites in one halo might lie in the same line of sight and be detected as clumps on one detection. On the other hand, the connection (through a spiral arm or tidal tail for example) between two parts of one galaxy might have such a low surface brightness that they are broken up into multiple detections or objects. In fact if you have noticed, exactly for this purpose, this is the only Signal to noise ratio that the user gives into NoiseChisel. The `true' detections and clumps can be objectively identified from the noise characteristics of the image, so you don't have to give any hand input Signal to noise ratio. @item --checksegmentation A file with the suffix @file{_seg.fits} will be created. This file keeps all the relevant steps in finding true clumps and segmenting the detections in various extensions. Having read the paper or the steps above, the extension name should be enough to understand which step each extension is showing. Examining this file can be an excellent guide in choosing the best set of parameters. Note that calling this function will significantly slow NoiseChisel. @end table @node NoiseChisel output, , NoiseChisel options, Invoking astnoisechisel @subsubsection NoiseChisel output The default name and directory of the outputs are explained in @ref{Automatic output}. NoiseChisel's default output (when none of the options starting with @option{--check} or the @option{--output} option are called) is one file ending with @file{_labeled.fits}. This file has the extensions listed below: @enumerate @item A copy of the input image, a copy is placed here for the following reasons: @itemize @item By flipping through the extensions, a user can check how accurate the detection and segmentation process was. @item All the inputs to MakeCatalog (see @ref{MakeCatalog}) are included in this one file which makes the running of MakeCatalog after NoiseChisel very easy. @item All masked pixels given to NoiseChisel will have a value of NaN in this image. So if you decide to run MakeCatalog after NoiseChisel, there is no more need to feed the mask image to MakeCatalog too. @end itemize @item The object labels. Each pixel in the input image is given a label in this extension, the labels start from one. The total number of labels is stored as the value to the @code{NOBJS} keyword in the header of this extension. It is also printed in verbose mode. @item The clump labels. All the pixels in the input image that belong to a true clump are given a positive label in this extension. The detected regions that were not a clump are given a negative value to clearly identify the noise from the detections. The total number of clumps in this image is stored in the @code{NCLUMPS} keyword of this extension and printed in verbose output. If the @option{--grownclumps} option is called, or a value of @code{1} is given to it in any of the configuration files, then instead of the original clump regions, the grown clumps will be stored in this extension. Note that if there is only one clump (or no clumps) over a detected region, then the whole detected region is given a label of 1. @item The final sky value on each pixel. See @ref{Sky value} for a complete explanation. See @ref{Grid interpolation and smoothing} for an explanation on the boxy appearance of this image. @item Similar to the previous mesh but for the standard deviation on each pixel. @end enumerate @node MakeCatalog, , NoiseChisel, Image analysis @section MakeCatalog Detecting and segmenting signal over an image results in labeled images where each pixel is labeled with the ID (an integer) that is specified by the detector program. But this labeled image by its self can hardly be of any scientific use. The job of MakeCatalog is to combine the input image, the noise properties and the labels of pixels into a catalog (a text file table) which can easily be used for high-level scientific interpretations. NoiseChisel (Gnuastro's signal detection tool, see @ref{NoiseChisel}) does not produce any catalog of the detected objects by its self. Only a labeled FITS image is output, see @ref{NoiseChisel output}. The output of NoiseChisel can be directly fed into MakeCatalog to generate the catalog. Some of the reasons for making the catalog in a separate program@footnote{Most existing software that do object detection also output a catalog, so this is not a common practice.} are listed below: @itemize @item Complexity: Adding in a catalog functionality to the detector program will add several more steps (and options) to its processing that can equally well be done outside of it. This makes following the code harder for a curious reader and also potentially adds bugs. Another advantage of less complexity is when the parameter you want to measure over one profile is not provided by the developers of MakeCatalog. You can simply open this tiny little program and add your desired calculation easily. In @ref{Adding new columns to MakeCatalog}, we have explained all the necessary steps to add a new column to MakeCatalog. However, if making a catalog was part of NoiseChisel, it would require a lot of energy to understand all the steps in order to add desired parameter. @item Low level nature of Gnuastro: Making catalogs is a separate process from labeling (detecting and segmenting) the pixels. A user might want to do certain operations on the labeled regions before creating a catalog for them. Another user might want the properties of the same pixels in another image (possibly from another broadband filter) for measuring the colors or SEDs for example. Here is an example of doing both: suppose you have images in various broad band filters at various resolutions and orientations. The image of one color will thus not lie exactly on another or even be in the same scale. However, it is imperative that the same pixels be used in measuring the colors of galaxies. Therefore NoiseChisel can be run on the reference image and ImageWarp (@ref{ImageWarp}) can be applied to the labeled images to find the pixels to use in the other image. Then MakeCatalog can generate the final catalog for both targets. It is currently customary to warp the images to the same pixel grid, however, this is very harmful for the data and creates correlated noise. It is much more accurate to do the transformations on the labeled image. @end itemize @menu * Quantifying data limits:: For comparing different catalogs. * Measuring elliptical parameters:: Estimating elliptical parameters. * Invoking astmkcatalog:: Options and arguments to MakeCatalog. * Adding new columns to MakeCatalog:: How to add new columns. @end menu @node Quantifying data limits, Measuring elliptical parameters, MakeCatalog, MakeCatalog @subsection Quantifying data limits @cindex Depth @cindex Clump magnitude limit @cindex Object magnitude limit @cindex Limit, object/clump magnitude @cindex Magnitude, object/clump detection limit Different datasets (images in the case of MakeCatalog) have different noise properties and different detection methods (or one method with a different set of parameters) will have different abilities to detect or measure certain kinds of objects in an image. Therefore it is very important to quantify our ability to detect and measure signal in noise. In this section we discuss these limits that are very important in any analysis. In astronomy, it is common to use the magnitude (a unit-less scale) and physical units, see @ref{Flux Brightness and magnitude}. Therefore all the measured discussed here are commonly defined in units of magnitudes. @table @asis @item Depth As we make more observations on one region of the sky and add the images over each other, we are able to decrease the standard deviation of the noise in each pixel@footnote{This is true for any noisy data, not just astronomical images}. Qualitatively, this decrease manifests its self by making fainter (per pixel) parts of the objects in the image more visible. Quantitatively, it increases the Signal to noise ratio, since the signal is fixed but the noise is decreased. It is very important to have in mind that here, noise is defined per pixel (or in the units of our data measurement), not per object. You can think of the noise as muddy water that is completely covering a flat ground@footnote{The ground is the sky value in this analogy, see @ref{Sky value}. Note that this analogy only holds for a flat sky value across the surface of the image or ground.} with some regions higher than the others@footnote{The peaks are (parts of) astronomical objects in this analogy.} in it. In this analogy, height is brightness. Let's assume that in your first observation the muddy water has just been stirred and you can't see anything through it. As you wait and make more observations, the mud settles down and the @emph{depth} of the transparent water increases as you wait. The summits of hills begin to appear. As the depth of clear water increases, the parts of the hills with lower heights (less surface brightness) can be seen more clearly. @cindex Depth The outputs of NoiseChisel include the Sky standard deviation (@mymath{\sigma}) on every group of pixels (a mesh) that were calculated from the undetected pixels in that mesh, see @ref{Tiling an image} and @ref{NoiseChisel output}. Let's take @mymath{\sigma_m} as the median @mymath{\sigma} over the successful meshes in the image (prior to interpolation or smoothing, see @ref{Grid interpolation and smoothing}). On different instruments pixels have different physical sizes (for example in micro-meters, or spatial angle over the sky), nevertheless, a pixel is our unit of data collection. In other words, while quantifying the noise, the physical or projected size of the pixels is irrelevant. We thus define the @emph{depth} of each data-set (or image) as the magnitude of @mymath{\sigma_m}. @cindex XDF @cindex CANDELS As an example, the XDF survey covers part of the sky that the Hubble space telescope has observed the most (for 85 orbits) and is consequently very small (@mymath{\sim4} arcmin@mymath{^2}). On the other hand, the CANDELS survey, is one of the widest multi-color surveys covering several fields (about 720 arcmin@mymath{^2}) but its deepest fields have only 9 orbits observation. The depth of the XDF and CANDELS-deep surveys in the near infrared WFC3/F160W filter are respectively 34.40 and 32.45 magnitudes. In a single orbit image, this same field has a depth of 31.32. Recall that a larger magnitude corresponds to less brightness, see @ref{Flux Brightness and magnitude}. @item Upper limit magnitude Due to the noisy nature of data, it is possible to get arbitrarily low values for a faint object's brightness (or arbitrarily high magnitudes). Given the scatter caused by the noise, such small values are meaningless: another similar depth observation will give a radically different value. This problem is most common when you use one image/filter to generate target labels (which specify which pixels belong to which object, see @ref{NoiseChisel output} and @ref{MakeCatalog}) and another image/filter to generate a catalog for measuring colors. The object might not be visible in the filter used for the latter image, or the image @emph{depth} (see above) might be much shallower. So you will get unreasonably faint magnitudes. For example when the depth of the image is 32 magnitudes, a measurement that gives a magnitude of 36 for a @mymath{\sim100} pixel object is clearly unreliable. In another similar depth image, we might measure a magnitude of 30 for it, and yet another might give 33. Furthermore, due to the noise scatter so close to the depth of the data-set, the total brightness might actually get measured as a negative value, so no magnitude can be defined (recall that a magnitude is a base-10 logarithm). @cindex Upper limit magnitude @cindex Magnitude, upper limit Using such unreliable measurements will directly affect our analysis, so we must not use them. However, all is not lost! Given our limited depth, there is one thing we can deduce about the object's magnitude: we can say that if something actually exists here (possibly buried deep under the noise), it must have a magnitude that is fainter than an @emph{upper limit magnitude}. To find this upper limit magnitude, we place the object's footprint (segmentation map) over random parts of the image where there are no detections, so we only have pure (possibly correlated) noise and undetected objects. Doing this a large number of times will give us a distribution of brightness values. The standard deviation (@mymath{\sigma}) of that distribution can be used to quantify the upper limit magnitude. @cindex Correlated noise Traditionally, faint/small object photometry was done using fixed circular apertures (for example with a diameter of @mymath{N} arc-seconds). In this way, the upper limit was like the depth discussed above: one value for the whole image. But with the much more advanced hardware and software of today, we can make customized segmentation maps for each object. The number of pixels (are of the object) used directly affects the final distribution and thus magnitude. Also the image correlated noise might actually create certain patters, so the shape of the object can also affect the result. So in MakeCatalog, the upper limit magnitude is found for each object in the image separately. Not one value for the whole image. @item Completeness limit @cindex Completeness As the surface brightness of the objects decreases, the ability to detect them will also decrease. An important statistic is thus the fraction of objects of similar morphology and brightness that will be identified with our detection algorithm/parameters in the given image. This fraction is known as completeness. For brighter objects, completeness is 1: all bright objects that might exist over the image will be detected. However, as we go to lower surface brightness objects, we fail to detect some and gradually we are not able to detect anything any more. For a given profile, the magnitude where the completeness drops below a certain level usually above @mymath{90\%} is known as the completeness limit. @cindex Purity @cindex False detections @cindex Detections false Another important parameter in measuring completeness is purity: the fraction of true detections to all true detections. In effect purity is the measure of contamination by false detections: the higher the purity, the lower the contamination. Completeness and purity are anti-correlated: if we can allow a large number of false detections (that we might be able to remove by other means), we can significantly increase the completeness limit. One traditional way to measure the completeness and purity of a given sample is by embedding mock profiles in regions of the image with no detection. However in such a study we must be really careful to choose model profiles as similar to the target of interest as possible. @end table @node Measuring elliptical parameters, Invoking astmkcatalog, Quantifying data limits, MakeCatalog @subsection Measuring elliptical parameters One of the most important class of parameters that are important for astronomical image analysis is the shape or morphology of the objects. In the case of galaxies (with a very rich variety of morphologies) studying the morphology of the detected objects is its self a is very complicated research subject which is a very active field of research now. So in this section, we will just discuss how the most basic morphological parameters are estimated: the elliptical parameters for a set of labeled pixels (that will be studied together and define our object of interest). These are: the major axis, the minor axis and the position angle along with the central position of the profile. The derivations below follow the SExtractor manual derivations but include more explanations. @cindex Moments Let's begin with one dimension for simplicity: Assume we have a set of @mymath{N} values (brightness for example) @mymath{B_i}, each at position @mymath{x_i}. The simplest parameter we can define is the geometric center of the object (@mymath{x_g}) (ignoring the brightness values): @mymath{x_g=(\sum_ix_i)/N}. @emph{Moments} are defined to incorporate both the value (brightness) and position of the data. The first moment can be written as: @dispmath{\overline{x}={\sum_iB_ix_i \over \sum_iB_i}} @cindex Variance @cindex Second moment @noindent This is essentially the weighted (by @mymath{B_i}) average position. The geometric center (@mymath{x_g}, defined above) is a special case of this with all @mymath{B_i=1}. The second moment is essentially the variance of the distributions: @dispmath{\overline{x^2}\equiv{\sum_i(B_ix_i-\overline{x})^2 \over \sum_iB_i} ={\sum_iB_i^2x_i^2 \over \sum_iB_i} - 2\overline{x}{\sum_iB_ix_i\over\sum_iB_i} + \overline{x}^2 ={\sum_iB_i^2x_i^2 \over \sum_iB_i} - \overline{x}^2} @cindex Standard deviation @noindent The last step was done from the definition of @mymath{\overline{x}}. So the square root of @mymath{\overline{x^2}} is the positional standard deviation (along the one-dimensional) of this particular brightness distribution (@mymath{B_i}). Crudely (or qualitatively), you can think of its square root as the distance (from @mymath{\overline{x}}) which contains a specific amount of the flux (depending on the @mymath{B_i} distribution). Similar to the first moment, the geometric second moment can be found by setting all @mymath{B_i=1}. So while the first moment quantified the position of the brightness distribution, the second moment quantifies how that brightness is dispersed about the first moment. In other words, it quantifies how ``sharp'' the object's image is. @cindex Floating point error Before continuing to two dimensions and the derivation of the elliptical parameters we will pause for an implementation technicality. You can ignore this paragraph if you don't want to implement these concepts. The basic definition (first fraction for @mymath{\overline{x^2}}) can be used without any major problem. However, using this fraction requires two runs over the data: one run to specify @mymath{\overline{x}} and one run for @mymath{\overline{x^2}}, this can be slow. However, using the last fraction above, we can estimate both the first and second moments in one run (since the @mymath{-\overline{x}^2} term can easily be added later). Using the last form creates a major technical issue however: due to the floating point accuracy. Suppose the object is located between pixels 10000 and 10020. While the object pixels are only distributed over 20 pixels (with a standard deviation @mymath{<20}), the mean has a value of @mymath{\sim10000}. The @mymath{\sum_iB_i^2x_i^2} will go to very very large values while the individual pixel differences will be much smaller, this will lower the accuracy of our calculation due to the limited accuracy of floating point operations. Since the variance only depends on the distance of each point from the mean, and for a constant/arbitrary @mymath{K}, @mymath{\overline{x-K}=\overline{x}-K}, we can calculate the second order moment using: @dispmath{\overline{x^2}={\sum_iB_i^2(x_i-K)^2 \over \sum_iB_i} - (\overline{x}-K)^2} @noindent The closer @mymath{K} is to @mymath{\overline{x}}, the better (the sums of squares will involve smaller numbers), as long as @mymath{K} is within the object limits (in the example above: @mymath{10000\leq{K}\leq10020}), the floating point error induced in our calculation will be negligible. For the most simplest implementation, in order to find the second moments (variance) in each dimension, MakeCatalog takes @mymath{K} to be the position of the first pixel that is assigned to the object under each dimension. Since @mymath{K} is arbitrary and an implementation/technical detail, we will ignore it for the remainder of this discussion. In two dimensions, the mean and variances can be written as: @dispmath{\overline{x}={\sum_iB_ix_i\over B_i}, \quad \overline{x^2}={\sum_iB_i^2x_i^2 \over \sum_iB_i} - \overline{x}^2} @dispmath{\overline{y}={\sum_iB_iy_i\over B_i}, \quad \overline{y^2}={\sum_iB_i^2y_i^2 \over \sum_iB_i} - \overline{y}^2} @dispmath{\quad\quad\quad\quad\quad\quad\quad\quad\quad \overline{xy}={\sum_iB_i^2x_iy_i \over \sum_iB_i} - \overline{x}\times\overline{y}} If an elliptical profile's major axis lies exactly along the @mymath{x} axis, then @mymath{\overline{x^2}} will be directly proportional with the major axis, @mymath{\overline{y^2}} with its minor axis and @mymath{\overline{xy}=0}. However, in reality we are not that lucky and (assuming galaxies can be parametrized as an ellipse) the major axis of galaxies can be in any direction on the image (in fact this is one of the core principles behind weak-lensing by shear estimation). So the purpose of the remainder of this section is to define a strategy to measure the position angle and axis ratio of some randomly positioned ellipses in an image, using the raw second moments that we have calculated above in our image coordinates. Let's assume we have rotated the galaxy by @mymath{\theta}, then the new second order moments can be written as: @dispmath{\overline{x_\theta^2} = \overline{x^2}\cos^2\theta + \overline{y^2}\sin^2\theta - 2\overline{xy}\cos\theta\sin\theta } @dispmath{\overline{y_\theta^2} = \overline{x^2}\sin^2\theta + \overline{y^2}\cos^2\theta + 2\overline{xy}\cos\theta\sin\theta} @dispmath{\overline{xy_\theta} = \overline{x^2}\cos\theta\sin\theta - \overline{y^2}\cos\theta\sin\theta + \overline{xy}(\cos^2\theta-\sin^2\theta)} We can now find the best @mymath{\theta} (@mymath{\theta_0}) such that the major axis lies along the @mymath{x_\theta} axis. This can be found by setting: @dispmath{\left.{\partial \overline{x_\theta^2} \over \partial \theta}\right|_{\theta_0}=0} Taking the derivative, we get: @dispmath{2\cos\theta_0\sin\theta_0(\overline{y^2}-\overline{x^2}) + 2(\cos^2\theta_0-\sin^2\theta_0)\overline{xy}=0} When @mymath{\overline{x^2}\neq\overline{y^2}}, we can write: @dispmath{\tan2\theta_0 = 2{\overline{xy} \over \overline{x^2}-\overline{y^2}}.} @cindex Position angle @noindent MakeCatalog uses the standard C math library's @code{atan2} function to estimate @mymath{\theta_0}, which we define as the position angle of the ellipse. To recall, this is the angle of the major axis of the ellipse with the @mymath{x} axis. By definition, when the elliptical profile is rotated by @mymath{\theta_0}, then @mymath{\overline{xy_{\theta_0}}=0}, @mymath{\overline{x_{\theta_0}^2}} will be the extent of the maximum variance and @mymath{\overline{y_{\theta_0}^2}} the extent of the minimum variance (which are perpendicular for an ellipse). Replacing @mymath{\theta_0} in the equations above for @mymath{\overline{x_\theta}} and @mymath{\overline{y_\theta}}, we can get the semi-major (@mymath{A}) and semi-minor (@mymath{B}) lengths: @dispmath{A^2\equiv\overline{x_{\theta_0}^2}= {\overline{x^2} + \overline{y^2} \over 2} + \sqrt{\left({\overline{x^2}-\overline{y^2} \over 2}\right)^2 + \overline{xy}^2}} @dispmath{B^2\equiv\overline{y_{\theta_0}^2}= {\overline{x^2} + \overline{y^2} \over 2} - \sqrt{\left({\overline{x^2}-\overline{y^2} \over 2}\right)^2 + \overline{xy}^2}} So as a summary, it is important to remember that the units of @mymath{A} and @mymath{B} are in pixels (same as the standard deviation) and that they represent the spatial light distribution of the object in both image dimensions if the object could be approximated as an ellipse. When the object cannot be represented as an ellipse, this interpretation breaks down: @mymath{\overline{xy_{\theta_0}}\neq0} and @mymath{\overline{y_{\theta_0}^2}} will not be the direction of minimum variance. @node Invoking astmkcatalog, Adding new columns to MakeCatalog, Measuring elliptical parameters, MakeCatalog @subsection Invoking MakeCatalog MakeCatalog will make a catalog from an input image and at least on labeled image. The executable name is @file{astmkcatalog} with the following general template @example $ astmkcatalog [OPTION ...] InputImage.fits @end example @noindent One line examples: @example $ astmkcatalog -mdri input.fits $ astmkcatalog --floatprecision=5 input.fits $ astmkcatalog --output=cat input_labeled.fits $ astmkcatalog --objlabs=K_labeled.fits --objhdu=1 \ --clumplabs=K_labeled.fits --clumphdu=2 i_band.fits @end example @cindex Gaussian @noindent If MakeCatalog is to do processing, an input image should be provided with the recognized extensions as input data, see @ref{Arguments}. Optionally a mask file can be specified to ignore some of the pixels in the image, see @ref{Mask image}. Note that if you generated the labeled image using NoiseChisel with a mask image as input, there is no more need to inform MakeCatalog of the mask image, see @ref{NoiseChisel output}. The options common to all Gnuastro programs are explained in @ref{Common options}. MakeCatalog needs 4 (or 5) images as input. These images can be separate extensions in one file (NoiseChisel's default output), or each can have its own file and its own extension. The full 5 images are listed in @ref{NoiseChisel output}. However, the clump labels image is not mandatory (when no clump catalog is required, for example in aperture photometry). When inspecting the object labels image, MakeProfiles will look for a @code{WCLUMPS} (short for with-clumps) header keyword. If that keyword is present and has a value of @code{yes} (not case sensitive, so @code{Yes}, or @code{YES} are also acceptable) then a clump image must also be provided and a clump catalog will be made. When @code{WCLUMPS} isn't present or has any other value, only an object catalog will be created and all clump related options will be ignored. @cindex Photometry, aperture @cindex Aperture photometry For example, if you only need an object catalog from NoiseChisel's output, you can use Header (see @ref{Header}) to modify or remove the @code{WCLUMPS} keyword in the objects HDU, then run MakeCatalog on it. Another example can be aperture photometry: let's assume you have made your labeled image (defining the apertures) with MakeProfiles. Clumps are not defined in this context, so besides the input and labeled image, you only need NoiseChisel's Sky and Sky standard deviation images. Since MakeProfile's output doesn't contain the @code{WCLUMPS} keyword, you just have to specify your labeled image with the @option{--objlabs} option and also set its HDU and no clumps catalog will be created. Note that labeled images have to be an integer type. Therefore, when using MakeProfiles to define the apertures/labels, you can use @option{--type=long} for example. When a clump catalog is also desired, two catalogs will be made: one for the objects (suffixed with @file{_o.txt}) and another for the clumps (suffixed with @file{_c.txt}). Therefore if any value is given to the @option{--output} option, MakeCatalogs will replace these two suffixes with any existing suffix in the given value. If no output value is given, MakeCatalog will use the input name, see @ref{Automatic output}. When only building an object catalog, any suffix in the value to output will just be replaced with @file{.txt}. The first set of options specify the properties of the inputs. Other necessary input images are treated very much like a mask image, see @ref{Mask image}. If no name is specified for them, their HDU is checked and if that differs from the input HDU, then there is no need to specify a file name for them. The object and column label images or segmentation maps should not be of a floating point type (@code{BITPIX}). @table @option @item -O @itemx --objlabs (@option{=STR}) The file name of the object labels, if in the same file as input, it is not mandatory. @item --objhdu (@option{=STR}) The HDU of the object labels image, the header keyword @code{NOBJS} must be present in this extension. The value to this keyword is used as the final number of objects and the number of rows in the output objects catalog. Only pixels with values above zero will be considered. @item -c @itemx --clumplabs (@option{=STR}) Similar to @option{--objlabs} but for the labels of the clumps. @item --clumphdu (@option{=STR}) Similar to @option{--objhdu}, but for the clumps. The @code{NCLUMPS} keyword in this header specifies the number of recognized clumps. @item -s @itemx --skyfilename (@option{=STR}) File name of an image keeping the Sky value for each pixel. @item --skyhdu (@option{=STR}) The HDU of the Sky value image. @item -t @itemx --stdfilename (@option{=STR}) File name of image keeping the Sky value standard deviation for each pixel. @item --stdhdu (@option{=STR}) The HDU of the Sky value standard deviation image. @item -z @itemx --zeropoint (@option{=FLT}) The zero point magnitude for the input image, see @ref{Flux Brightness and magnitude}. @item -E @itemx --skysubtracted If the image has already been sky subtracted by another program, then you need to notify MakeCatalog through this option. Note that this is only relevant when the Signal to noise ratio is to be calculated. @item -T @itemx --threshold (@option{=FLT}) For all the columns, only consider pixels that are above a given relative threshold. Symbolizing the value of this option as @mymath{T}, the Sky for a pixel at @mymath{(i,j)} with @mymath{\mu_{ij}} and its Standard deviation with @mymath{\sigma_{ij}}, that pixel will only be used if its value (@mymath{B_{ij}}) satisfies this condition: @mymath{B_{ij}>\mu_{ij}+{T}\sigma_{ij}}. The only calculations that will not be affected are is the average river values (@option{--riverave}), since they are used as a reference. A commented row will be added in the header of the output catalog that will print the given value, since this is a very important issue, it starts with @command{**IMPORTANT**}. NoiseChisel will detect very diffuse signal which is useful in most cases where the aggregate properties of the detections are desired, since there is signal there (with the desired certainty). However, in some cases, only the properties of the peaks of the objects/clumps are desired, for example in attempting to separate stars from galaxies, the peaks are the major target and the diffuse regions only act to complicate the separation. With this option, MakeCatalog will simply ignore any pixel below the relative threshold. @cindex NaN This option is not mandatory, so if it isn't given (after reading the command-line and all configuration files, see @ref{Configuration files}), MakeCatalog will still operate. However, if it has a value in any lower-level configuration file and you want to ignore that value for this particular run or in a higher-level configuration file, then set it to NaN, for example @option{--threshold=nan}. Gnuastro uses the C library's @code{strtod} function to read floats, which is not case-sensative in reading NaN values. But to be consistent, it is good practice to only use @option{nan}. @end table @noindent Through the next group of options, you can customize the general output plain text catalog. The basic idea behind the options about the width and precision of the different types is the fact that some columns don't need too much space, while some do. The width is the number of text columns given to data of each type in the output plain text catalog. The precision is the number of digits to show after the decimal point in floating point numbers. We have defined two types of floating point numbers here, one is for less accurate precision, like magnitude, while the other is used when more accuracy is necessary. A common example of the latter is right ascension and declination. These variables usually need to be printed with more than 6 point accuracy. Note that all the values are calculated and stored internally as double precision floating point numbers, the distinction made here is only for printing them. @table @option @item --nsigmag (@option{=FLT}) The magnitude of the value to this option multiplied by the maximum standard deviation over the objects or clumps is reported in the output catalog. This value is a per-pixel value, not per object and is not found over an area or aperture, like the common @mymath{5\sigma} values that are commonly reported as a measure of depth. They are based on a certain area and are relics from the time of analog data collection and processing. Modern tools use digital imaging detectors and the area is that of a pixel. @item --intwidth (@option{=INT}) The width of printing the integer values. In MakeCatalog, all IDs, numbers (counters) and areas are considered to be an integer. @item --floatwidth (@option{=INT}) The width of a normal precision floating point column. Any column that is not designated in @option{--intwidth} or @option{--accuwidth} is considered to be a normal precision floating point. @item --accuwidth (@option{=INT}) The width columns to be printed with extra accuracy. In MakeCatalog the following columns are printed with extra accuracy: right ascension, declination, brightness, river pixel averages (see Akhlaghi and Ichikawa 2015 for the definition of river pixels), the sky and the sky standard deviation. @item --floatprecision (@option{=INT}) The number of digits to the right of the decimal point in normal floating point display. @item --accuprecision (@option{=INT}) The number of digits to the right of the decimal point in more accurate floating point display. @end table The upper limit magnitude was discussed in @ref{Quantifying data limits}. Unlike other measured values/columns in MakeCatalog, the upper limit magnitude needs several defined parameters which are discussed here. All the upper limit magnitude specific options start with @option{up} for upper limit, except for @option{--envseed} that is also present in other programs and is general for any job requiring random number generation. @cindex Reproducibility One very important consideration in Gnuastro is reproducibility. Therefore, the values to all of these parameters along with others (like the random number generator type and seed) are also reported in the comments of the final catalog when the upper limit magnitude column is desired. One of those parameters is the number of threads used in this run of MakeCatalog. This might seem irrelevant. The job of sampling a large number of positions over the image is an ``embarrasingly parallel'' kind of problem which can greatly benefit from threads. For maximum efficiency, the objects in the catalog are divided between the threads and the random number generator is used independently on each thread. So even when the random number generator type and seed are identical, if the number of threads differ, you will get different results. Ofcourse, the difference is due to scatter and is statistically negligible, but it is not exactly reproducible (which is important in some contexts). @table @option @item --upmask (@option{=STR}) File name of mask image to use for upper-limit calculation. In some cases (especially when doing matched photometry), the object labels specified in the main input and mask image might not be adequate. In other words they do not necessarily have to cover @emph{all} detected objects: the user might have selected only a few of the objects in their labeled image. All the non-zero pixels of the image specified by this option (in the @option{--upmaskhdu} extension) will be set as blank for the upper limit magnitude calculation. For example, when you are using labels from another image, you can give NoiseChisel's objects image output for this image as the value to this option. In this way, you can be sure that regions with data do not harm your distribution. See @ref{Quantifying data limits} for more on the upper limit magnitude. @item --upmaskhdu (@option{=STR}) The extension in the file specified by @option{--upmask}. @item --upnum (@option{=INT}) The number of random samples to take for all the objects. A larger value to this option will give a more accurate result (assymptotically), but it will also slow down the process. When a randomly positioned sample overlaps with a detected/masked pixel it is not counted and another random position is found until the object completely lies over an undetected region. So you can be sure that for each object, this many samples over undetected objects are made. See the upper limit magnitude discussion in @ref{Quantifying data limits} for more. @item --envseed Read the random number generator type and seed value from the environment (see @ref{Generating random numbers}). Random numbers are used in calculating the random positions of different samples of each object. @item --upsclipmultip (@option{=FLT}) The multiple of @mymath{\sigma} to use in @mymath{\sigma}-clipping the final distribution (see @ref{Sigma clipping}). The images might have some artifacts or some regions with signal in the image might not have been removed correctly. If a random sampling falls over such regions, they can significantly bias the final standard deviation. To avoid the effect of such outliers, after the distribution is found, it is @mymath{\sigma}-clipped (by convergence). @item --upsclipaccu (@option{=FLT}) Relative difference between two successive @mymath{\sigma} measurements to halt the @mymath{\sigma}-clipping process by convergence, see the explanations for @option{--upsclipmultip} for more. @item --upnsigma (@option{=FLT}) The multiple of the standard deviation (or @mymath{\sigma}) used to measure the magnitude. Note that this is the final @mymath{\sigma} produced after the @mymath{\sigma}-clipping. @end table The final group of options particular to MakeCatalog are those that specify which columns should be displayed in the output catalogs. For each column there is an option, if it has been called on the command line or in any of the configuration files, it will included as a column in the output catalog. Some of the options apply to both objects and clumps and some are particular to only one of them. The latter cases are explicitly marked with [Objects] or [Clumps] to specify the catalog they will be placed in. The order of the columns in the output catalog is the inverse of the order their options are read in. For example see the following command@footnote{This command is practically identical to the first command in the one-line examples, see @ref{Options} for an explanation of the concatenation of the on/off options.}: @example $ astmkcatalog --magnitude --dec --ra --id input.fits @end example @noindent In this example, if no columns are specified in any of the configuration files (see @ref{Configuration files}), then the columns in the catalogs produced by this command will have the following order: ID, RA, Dec and Magnitude. Contrary to what it looks like, this is done to make life easier for the users. The configuration files can also keep any of the columns (so you don't have to specify your desired columns every time). This inverse ordering thus comes from their precedence, see @ref{Configuration file precedence}. For example catalogs usually have at least an ID column and position columns (in the image and/or the world coordinate system). By reading the order of the columns in reverse you can have your fixed set of columns in your system wide configuration file and in any particular run, if you want some other information about objects or clumps, you can add those columns on the command-line. Through the user and current directory configuration files, you can also have custom catalogs in each of your working directories, without bothering to specify the columns every time you run MakeCatalog in those directories. @table @option @item --i @itemx --id The ID of the clump or object. @item -j @itemx hostobjid [Clumps] The ID of the object which hosts this clump. @item -I @itemx --idinhostobj [Clumps] The ID of this clump in its host object. @item -C @itemx --numclumps [Objects] The number of clumps in this object. @item -a @itemx --area The area (number of pixels) in any clump or object. @item --clumpsarea [Objects] The total area of all the clumps in this object. @item -x @itemx --x The flux weighted center of all objects and clumps along the first FITS axis (horizontal when viewed in SAO ds9). The weight has to have a positive value (pixel value larger than the Sky value) to be meaningful! Specially when doing matched photometry, this might not happen: no pixel value might be above the Sky value. In such cases, where there was no pixel with a value larger than the Sky in the object or clump, the geometric center (ignoring pixel values, only their positions) over the object or clump is used instead of the flux weighted center (see @option{--geox}). @item -y @itemx --y The flux weighted center of all objects and clumps along the second FITS axis (vertical when viewed in SAO ds9). See @option{--x}. @item --geox The geometric center of all objects and clumps along the first FITS axis axis. The geometric center is the average pixel positions irrespective of their pixel values. @item --geoy The geometric center of all objects and clumps along the second FITS axis axis, see @option{--geox}. @item --clumpsx [Objects] The flux weighted center of all the clumps in this object along the first FITS axis. See @option{--x}. @item --clumpsy [Objects] The flux weighted center of all the clumps in this object along the second FITS axis. See @option{--x}. @item --clumpsgeox [Objects] The geometric center of all the clumps in this object along the first FITS axis. See @option{--geox}. @item --clumpsgeoy [Objects] The geometric center of all the clumps in this object along the second FITS axis. See @option{--geox}. @item -r @itemx --ra Flux weighted right ascension of all objects or clumps, see @option{--x}. @item -d @itemx --dec Flux weighted declination of all objects or clumps, see @option{--x}. @item --geora Geometric center right ascension of all objects or clumps, see @option{--geox}. @item --geodec Geometric center declination of all objects or clumps, see @option{--geox}. @item --clumpsra [Objects] Flux weighted right ascension of all clumps in this object, see @option{--x}. @item --clumpsdec [Objects] Flux weighted declination of all clumps in this object, see @option{--x}. @item --clumpsgeora [Objects] Geometric center right ascension of all clumps in this object, see @option{--geox}. @item --clumpsgeodec [Objects] Geometric center declination of all clumps in this object, see @option{--geox}. @item -b @itemx --brightness The brightness (sum of all pixel values), see @ref{Flux Brightness and magnitude}. For each clump in the clumps catalog, the ambient brightness (flux of river pixels around the clump multiplied by the area of the clump) is removed, see @option{--riverflux}. So the sum of clump brightnesses in the clump catalog will be smaller than the total clump brightness in the @option{--clumpbrightness} column of the objects catalog. @item --clumpbrightness [Objects] The total brightness of the clumps within an object. This is simply the sum of the pixels associated with clumps in the object. @item --noriverbrightness [Clumps] The Sky (not river) subtracted clump brightness. By definition, for the clumps, the average brightness of the rivers surrounding it are subtracted from it for a first order accounting for contamination by neighbors. In cases where you will be calculating the flux brightness difference later (one example below) the contamination will be (mostly) removed at that stage, which is why this column was added. One example might be this: you want to know the change in the clump flux as a function of threshold (see @option{--threshold}). So you will make two catalogs (each having this column but with different thresholds) and then subtract the lower threshold catalog (higher brightness) from the higher threshold catalog (lower brightness). The effect is most visible when the rivers have a high average signal-to-noise ratio. The removed contribution from the pixels below the threshold will be less than the river pixels. Therefore the river-subtracted brightness (@option{--brightness}) for the thresholded catalog for such clumps will be larger than the brightness with no threshold! @item -m @itemx --magnitude The magnitude of clumps or objects, see @option{--brightness}. @item -e @itemx --magnitudeerr The magnitude error of clumps or objects. The magnitude error is calculated from the signal-to-noise ratio (see @option{--sn}, abbreviated as @mymath{S}): @mymath{\Delta{M}=2.5/(S\times\ln{10})}. Note that until now this error assumes un-correlated pixel values and also does not include the error in estimating the aperture (or error in generating the labeled image). For now these factors have to be found by other means. @url{https://savannah.gnu.org/task/index.php?14124, Task 14124} has been defined for work on adding these sources of error too. @item --clumpsmagnitude [Objects] The magnitude of all clumps in this object, see @option{--clumpbrightness}. @item --upperlimitmag [Objects] The upper limit magnitude for this object. The object's footprint is used over randomly positioned parts of the image that do not cover a detected object. The standard deviation of the final distribution is then the upper limit magnitude, see @ref{Quantifying data limits} for a complete explanation. This is very important for the fainter objects in the image where the measured magnitudes are not reliable. @item --riverave [Clumps] The average brightness of the river pixels around this clump. River pixels were defined in Akhlaghi and Ichikawa 2015. In short they are the pixels immediately outside of the clumps. This value is used internally to find the brightness (or magnitude) and signal to noise ratio of the clumps. It can generally also be used as a scale to gauge the base (ambient) flux surrounding the clump. In case there was no river pixels, then this column will have the value of the Sky under the clump. So note that this value is @emph{not} sky subtracted. @item --rivernum [Clumps] The number of river pixels around this clump, see @option{--riverflux}. @item -n @itemx --sn The Signal to noise ratio (S/N) of all clumps or objects. See Akhlaghi and Ichikawa (2015) for the exact equations used. @item --sky The sky flux (per pixel) value under this object or clump. This is actually the mean value of all the pixels in the sky image that lie on the same position as the object or clump. @item --std The sky value standard deviation (per pixel) for this clump or object. Like @option{--sky}, this is the average of the values in the input sky standard deviation image pixels that lie over this object. @item -A @itemx --semimajor The pixel-value weighted semi-major axis of the profile (assuming it is an ellipse) in units of pixels. @item -B @itemx --semiminor The pixel-value weighted semi-minor axis of the profile (assuming it is an ellipse) in units of pixels. @item -p @itemx --positionangle The pixel-value weighted angle of the semi-major axis with the first FITS axis in degrees. @item --geosemimajor The geometric (ignoring pixel values) semi-major axis of the profile, assuming it is an ellipse. @item --geosemiminor The geometric (ignoring pixel values) semi-minor axis of the profile, assuming it is an ellipse. @item --geopositionangle The geometric (ignoring pixel values) angle of the semi-major axis with the first FITS axis in degrees. @end table @node Adding new columns to MakeCatalog, , Invoking astmkcatalog, MakeCatalog @subsection Adding new columns to MakeCatalog The common development characteristics of MakeCatalog and other Gnuastro programs is explained in @ref{Developing}. This section might be more clearly understood after reading that chapter. MakeCatalog has been designed to allow easy addition of new columns, here we will give a fast over-view of the steps you need to take to define a new output column. After adding and testing your column, you are most welcome (and encouraged) to share it with us so we can add to the next release of Gnuastro for everyone else to also benefit from your efforts. MakeCatalog will first have two passes over the input pixels: in the first pass it will gather mainly object information and in the second run, it will mainly focus on the clumps, or any other measurement that needs an output from the first pass. These two passes are designed to be raw summations: no extra processing. This will allow parallel processing and simplicity/clarity. Once the passes are done, depending on the order of options that the user has defined the appropriate function will be called to add a processed column from the raw calculations to the output array (which will be printed). So if your new calculation, needs new raw information from the pixels, then you will need to also modify the respective @code{firstpass} and @code{secondpass} functions and define new information table columns in @file{main.h}. For all the steps below, it is easiest to just copy and paste an existing option and change the variables in each step. In all these different places, the options are sorted in the same order (same order as @ref{Invoking astmkcatalog}). This allows a particular column/option to be easily found in all steps. Therefore in adding your new option, be sure to keep it in the same relative place in the list in all the separate places (it doesn't necessarily have to be in the end), and near conceptually similar options. @table @file @item main.h The @code{objectcols} and @code{clumpcols} enumerated variables (@code{enum}) define the labels for the separate information table columns (the raw pixel calculations). If your new calculation requires new raw columns, the add new macros for them. The @code{outcols} enumerated variables define the recognized output columns. You will need to add a new name for your desired column here, then add a row for your new parameter in the @code{uiparams} structure, the name should be the same as the one you used in @code{outcols} (in small caps). @cindex GNU C library @item args.h This file specifies all the parameters for the GNU C library, Argp structure that is in charge of reading the user's options. It is best that the option name be the same as the name you put in @code{outcols} (in @file{main.h}), like the other options that are already defined. Define a new option in @code{argp_option} (rows between the @code{@{} and @code{@}}). The first is the name of the option, the second is its short option name (see @ref{Options}). The next two values should be @code{0} and the last should be a short description of your option/column. For the second element is best to use a number (so no short option is defined for the user) which in Gnuastro is defined to be a number larger than 500. The range of used numbers (and short option names) are shown in the comment immediately above @code{argp_option} structure, increase that number by one and use that number for your new option. Go down to the @code{parse_opt} function and add a @code{case} for your specific option (using the same number you specified above), then update the contents, based on the new macros you defined @code{main.h}. @item ui.c In the @code{readconfig} function, add an @code{else if} for your option (easiest to just copy and paste, then update). In the @code{printvalues} function's @code{switch} structure, add a @code{case} for your option. Finally, in the @code{preparearrays} function, add a @code{case} for your new output column. Note that if the column is to be used for both objects and clumps, you need to set both @code{p->objcols} and @code{p->clumpcols}. @item mkcatalog.c If your procedure needs new raw calculations, add a new line to appropriate parts of the @code{firstpass}, and/or @code{secondpass} functions, they should be clear and are fully commented. Then add a @code{case} for your column in the @code{makeoutput} function, here you will need to call a function (which should be defined in @file{columns.c}). @item columns.c Define the function that will write your desired column in the output column using the raw input calculations here. There are a lot of functions in this file which you can use to model and they are commented, in short you have to specify a header (commented column), the units of your variable, the possible accuracy to print and finally the actual columns. @end table @node Modeling and fittings, High-level calculations, Image analysis, Top @chapter Modeling and fitting @cindex Fitting @cindex Modeling In order to fully understand observations after initial analysis on the image, it is very important to compare them with the existing models to be able to further understand both the models and the data. The tools in this chapter create model galaxies and will provide 2D fittings to be able to understand the detections. @menu * MakeProfiles:: Making mock galaxies and stars. * MakeNoise:: Make (add) noise to an image. @end menu @node MakeProfiles, MakeNoise, Modeling and fittings, Modeling and fittings @section MakeProfiles @cindex Checking detection algorithms @pindex @r{MakeProfiles (}astmkprof@r{)} MakeProfiles will create mock astronomical profiles from a catalog, either individually or together in one output image. In data analysis, making a mock image can act like a calibration tool, through which you can test how successfully your detection technique is able to detect a known set of objects. There are commonly two aspects to detecting: the detection of the fainter parts of bright objects (which in the case of galaxies fade into the noise very slowly) or the complete detection of an over-all faint object. Making mock galaxies is the most accurate (and idealistic) way these two aspects of a detection algorithm can be tested. You also need mock profiles in fitting known functional profiles with observations. MakeProfiles was initially built for extra galactic studies, so currently the only astronomical objects it can produce are stars and galaxies. We welcome the simulation of any other astronomical object. The general outline of the steps that MakeProfiles takes are the following: @enumerate @item Build the full profile out to its truncation radius in a possibly over-sampled array. @item Multiply all the elements by a fixed constant so its total magnitude equals the desired total magnitude. @item If @option{--individual} is called, save the array for each profile to a FITS file. @item If @option{--nomerged} is not called, add the overlapping pixels of all the created profiles to the output image and abort. @end enumerate Using input values, MakeProfiles adds the World Coordinate System (WCS) headers of the FITS standard to all its outputs (except PSF images!). For a simple test on a set of mock galaxies in one image, there is no need for the third step or the WCS information. @cindex Transform image @cindex Lensing simulations @cindex Image transformations However in complicated simulations like weak lensing simulations, where each galaxy undergoes various types of individual transformations based on their position, those transformations can be applied to the different individual images with other programs. After all the transformations are applied, using the WCS information in each individual profile image, they can be merged into one output image for convolution and adding noise. @menu * Modeling basics:: Astronomical modeling basics. * If convolving afterwards:: Considerations for convolving later. * Flux Brightness and magnitude:: About these measures of energy. * Profile magnitude:: Definition of total profile magnitude. * Invoking astmkprof:: Inputs and Options for MakeProfiles. @end menu @node Modeling basics, If convolving afterwards, MakeProfiles, MakeProfiles @subsection Modeling basics In the subsections below, first a review of some very basic information and concepts behind modeling a real astronomical image is given. You can skip this subsection if you are already sufficiently familiar with these concepts. @menu * Defining an ellipse:: Defining an ellipse in 2D. * PSF:: Radial profiles for the PSF. * Stars:: Making mock star profiles. * Galaxies:: Radial profiles for galaxies. * Sampling from a function:: Sample a function on a pixelated canvas. * Oversampling:: Oversampling the model. @end menu @node Defining an ellipse, PSF, Modeling basics, Modeling basics @subsubsection Defining an ellipse @cindex Ellipse The PSF, see @ref{PSF}, and galaxy radial profiles are generally defined on an ellipse so in this section first defining an ellipse on a pixelated 2D surface is discussed. Labeling the major axis of an ellipse @mymath{a}, and its minor axis with @mymath{b}, the axis ratio is defined as: @mymath{q\equiv b/a}. The major axis of an ellipse can be aligned in any direction, therefore define the angle of the major axis to the horizontal axis of the image is defined to be the position angle of the ellipse and in this book, we show it with @mymath{\theta}. @cindex Radial profile on ellipse Our aim is to put a radial profile of any functional form @mymath{f(r)} over an ellipse. Let's define the radial distance @mymath{r_{el}} as the distance on the major axis to the center of the ellipse which is located at @mymath{x_c} and @mymath{y_c}. We want to find the elliptical distance of a point located at @mymath{(i,j)}, in the image coordinate system, from the center of the ellipse. First the coordinate system is rotated by @mymath{\theta} to get the new rotated coordinates of that point @mymath{(i_r,j_r)}: @dispmath{i_r(i,j)=(i_c-i)\cos(\theta)+(j_c-j)\sin(\theta)} @dispmath{j_r(i,j)=(j_c-j)\cos(\theta)-(i_c-i)\sin(\theta)} @cindex Elliptical distance @noindent The elliptical distance of a point located at @mymath{(i,j)} can now be defined as: @mymath{r_{el}^2=\sqrt{i_r^2+j_r^2/q^2} }. To place the radial profiles explained below over an ellipse, @mymath{f(r_{el}(i,j))} is calculated based on the functional radial profile desired. @cindex Breadth first search @cindex Inside-out construction @cindex Making profiles pixel by pixel @cindex Pixel by pixel making of profiles The way MakeProfiles builds the profile is that the nearest pixel in the image to the given profile center is found and the profile value is calculated for it, see @ref{Sampling from a function}. The next pixel which the profile value is calculated on is the next nearest neighbor of the initial pixel to the profile center (as defined by @mymath{r_{el}}). This is done fairly efficiently using a breadth first parsing strategy@footnote{@url{http://en.wikipedia.org/wiki/Breadth-first_search}} which is implemented through an ordered linked list. Using this approach, we only go over one layer of pixels on the circumference of the profile to build the profile. Not one more extra pixel has to be checked. Another consequence of this strategy is that extending MakeProfiles to three dimensions becomes very simple: only the neighbors of each pixel have to be changed. Everything else after that (when the pixel index and its radial profile have entered the linked list) is the same, no matter the number of dimensions we are dealing with. @node PSF, Stars, Defining an ellipse, Modeling basics @subsubsection Point Spread Function @cindex PSF @cindex Point source @cindex Diffraction limited @cindex Point Spread Function @cindex Spread of a point source Assume we have a `point' source, or a source that is far smaller than the maximum resolution (a pixel). When we take an image of it, it will `spread' over an area. To quantify that spread, we can define a `function'. This is how the point spread function or the PSF of an image is defined. This `spread' can have various causes, for example in ground based astronomy, due to the atmosphere. In practice we can never surpass the `spread' due to the diffraction of the lens aperture. Various other effects can also be quantified through a PSF. For example, the simple fact that we are sampling in a discrete space, namely the pixels, also produces a very small `spread' in the image. @cindex Blur image @cindex Convolution @cindex Image blurring @cindex PSF image size Convolution is the mathematical process by which we can apply a `spread' to an image, or in other words blur the image, see @ref{Convolution process}. The Brightness of an object should remain unchanged after convolution, see @ref{Flux Brightness and magnitude}. Therefore, it is important that the sum of all the pixels of the PSF be unity. The PSF image also has to have an odd number of pixels on its sides so one pixel can be defined as the center. In MakeProfiles, the PSF can be set by the two methods explained below. @table @asis @item Parametric functions @cindex FWHM @cindex PSF width @cindex Parametric PSFs @cindex Full Width at Half Maximum A known mathematical function is used to make the PSF. In this case, only the parameters to define the functions are necessary and MakeProfiles will make a PSF based on the given parameters for each function. In both cases, the center of the profile has to be exactly in the middle of the central pixel of the PSF (which is automatically done by MakeProfiles). When talking about the PSF, usually, the full width at half maximum or FWHM is used as a scale of the width of the PSF. @table @cite @item Gaussian @cindex Gaussian distribution In the older papers, and to a lesser extent even today, some researchers use the 2D Gaussian function to approximate the PSF of ground based images. In its most general form, a Gaussian function can be written as: @dispmath{f(r)=a \exp \left( -(x-\mu)^2 \over 2\sigma^2 \right)+d} Since the center of the profile is pre-defined, @mymath{\mu} and @mymath{d} are constrained. @mymath{a} can also be found because the function has to be normalized. So the only important parameter for MakeProfiles is the @mymath{\sigma}. In the Gaussian function we have this relation between the FWHM and @mymath{\sigma}: @cindex Gaussian FWHM @dispmath{\rm{FWHM}_g=2\sqrt{2\ln{2}}\sigma \approx 2.35482\sigma} @item Moffat @cindex Moffat function The Gaussian profile is much sharper than the images taken from stars on photographic plates or CCDs. Therefore in 1969, Moffat proposed this functional form for the image of stars: @dispmath{f(r)=a \left[ 1+\left( r\over \alpha \right)^2 \right]^{-\beta}} @cindex Moffat beta Again, @mymath{a} is constrained by the normalization, therefore two parameters define the shape of the Moffat function: @mymath{\alpha} and @mymath{\beta}. The radial parameter is @mymath{\alpha} which is related to the FWHM by @cindex Moffat FWHM @dispmath{\rm{FWHM}_m=2\alpha\sqrt{2^{1/\beta}-1}} @cindex Compare Moffat and Gaussian @cindex PSF, Moffat compared Gaussian @noindent Comparing with the PSF predicted from atmospheric turbulence theory with a Moffat function, Trujillo et al.@footnote{Trujillo, I., J. A. L. Aguerri, J. Cepa, and C. M. Gutierrez (2001). ``The effects of seeing on S@'ersic profiles - II. The Moffat PSF''. In: MNRAS 328, pp. 977---985.} claim that @mymath{\beta} should be 4.765. They also show how the Moffat PSF contains the Gaussian PSF as a limiting case when @mymath{\beta\to\infty}. @end table @item An input FITS image An input image file can also be specified to be used as a PSF. If the sum of its pixels are not equal to 1, the pixels will be multiplied by a fraction so the sum does become 1. @end table While the Gaussian is only dependent on the FWHM, the Moffat function is also dependent on @mymath{\beta}. Comparing these two functions with a fixed FWHM gives the following results: @itemize @item Within the FWHM, the functions don't have significant differences. @item For a fixed FWHM, as @mymath{\beta} increases, the Moffat function becomes sharper. @item The Gaussian function is much sharper than the Moffat functions, even when @mymath{\beta} is large. @end itemize @node Stars, Galaxies, PSF, Modeling basics @subsubsection Stars @cindex Modeling stars @cindex Stars, modeling In MakeProfiles, stars are generally considered to be a point source. This is usually the case for extra galactic studies, were nearby stars are also in the field. Since a star is only a point source, we assume that it only fills one pixel prior to convolution. In fact, exactly for this reason, in astronomical images the light profiles of stars are one of the best methods to understand the shape of the PSF and a very large fraction of scientific research is preformed by assuming the shapes of stars to be the PSF of the image. @node Galaxies, Sampling from a function, Stars, Modeling basics @subsubsection Galaxies @cindex Galaxy profiles @cindex S@'ersic profile @cindex Profiles, galaxies @cindex Generalized de Vaucouleur profile Today, most practitioners agree that the flux of galaxies can be modeled with one or a few generalized de Vaucouleur's (or S@'ersic) profiles. @dispmath{I(r) = I_e \exp \left ( -b_n \left[ \left( r \over r_e \right)^{1/n} -1 \right] \right )} @cindex Brightness @cindex S@'ersic, J. L. @cindex S@'ersic index @cindex Effective radius @cindex Radius, effective @cindex de Vaucouleur profile @cindex G@'erard de Vaucouleurs G@'erard de Vaucouleurs (1918-1995) was first to show in 1948 that this function best fits the galaxy light profiles, with the only difference that he held @mymath{n} fixed to a value of 4. 20 years later in 1968, J. L. S@'ersic showed that @mymath{n} can have a variety of values and does not necessarily need to be 4. This profile depends on the effective radius (@mymath{r_e}) which is defined as the radius which contains half of the profile brightness (see @ref{Profile magnitude}). @mymath{I_e} is the flux at the effective radius. The S@'ersic index @mymath{n} is used to define the concentration of the profile within @mymath{r_e} and @mymath{b_n} is a constant dependent on @mymath{n}. MacArthur et al.@footnote{MacArthur, L. A., S. Courteau, and J. A. Holtzman (2003). ``Structure of Disk-dominated Galaxies. I. Bulge/Disk Parameters, Simulations, and Secular Evolution''. In: ApJ 582, pp. 689---722.} show that for @mymath{n>0.35}, @mymath{b_n} can be accurately approximated using this equation: @dispmath{b_n=2n - {1\over 3} + {4\over 405n} + {46\over 25515n^2} + {131\over 1148175n^3}-{2194697\over 30690717750n^4}} @node Sampling from a function, Oversampling, Galaxies, Modeling basics @subsubsection Sampling from a function @cindex Sampling A pixel is the ultimate level of accuracy to gather data, we can't get any more accurate in one image, this is known as sampling in signal processing. However, the mathematical profiles which describe our models have infinite accuracy. Over a large fraction of the area of astrophysically interesting profiles (for example galaxies or PSFs), the variation of the profile over the area of one pixel is not too significant. In such cases, the elliptical radius (@mymath{r_{el}} of the center of the pixel can be assigned as the final value of the pixel, see @ref{Defining an ellipse}). @cindex Integration over pixel @cindex Gradient over pixel area @cindex Function gradient over pixel area As you approach their center, some galaxies become very sharp (their value significantly changes over one pixel's area). This sharpness increases with smaller effective radius and larger S@'ersic values. Thus rendering the central value extremely inaccurate. The first method that comes to mind for solving this problem is integration. The functional form of the profile can be integrated over the pixel area in a 2D integration process. However, unfortunately numerical integration techniques also have their limitations and when such sharp profiles are needed they can become extremely inaccurate. @cindex Monte carlo integration The most accurate method of sampling a continuous profile on a discrete space is by choosing a large number of random points within the boundaries of the pixel and taking their average value (or Monte Carlo integration). This is also, generally speaking, what happens in practice with the photons on the pixel. The number of random points can be set with @option{--numrandom}. Unfortunately, repeating this Monte Carlo process would be extremely time and CPU consuming if it is to be applied to every pixel. In order to not loose too much accuracy, in MakeProfiles, the profile is built using both methods explained above. The building of the profile begins from its central pixel and continues outwards. Monte Carlo integration is first applied (which yields @mymath{F_r}), then the central pixel value (@mymath{F_c}) on the same pixel. If the fractional difference (@mymath{|F_r-F_c|/F_r}) is lower than a given tolerance level we will stop using Monte Carlo integration and only use the central pixel value. @cindex Inside-out construction The ordering of the pixels in this inside-out construction is based on @mymath{r=\sqrt{(i_c-i)^2+(j_c-j)^2}}, not @mymath{r_{el}}, see @ref{Defining an ellipse}. When the axis ratios are large (near one) this is fine. But when they are small and the object is highly elliptical, it might seem more reasonable to follow @mymath{r_{el}} not @mymath{r}. The problem is that the gradient is stronger in pixels with smaller @mymath{r} (and larger @mymath{r_{el}}) than those with smaller @mymath{r_{el}}. In other words, the gradient is strongest along the minor axis. So if the next pixel is chosen based on @mymath{r_{el}}, the tolerance level will be reached sooner and lots of pixels with large fractional differences will be missed. Monte Carlo integration uses a random number of points. Thus, every time you run it, by default, you will get a different distribution of points to sample within the pixel. In the case of large profiles, this will result in a slight difference of the pixels which use Monte Carlo integration each time MakeProfiles is run. To have a deterministic result, you have to fix the random number generator properties which is used to build the random distribution. This can be done by setting the @code{GSL_RNG_TYPE} and @code{GSL_RNG_SEED} environment variables and calling MakeProfiles with the @option{--envseed} option. To learn more about the process of generating random numbers, see @ref{Generating random numbers}. The seed values are fixed for every profile: with @option{--envseed}, all the profiles have the same seed and without it, each will get a different seed using the system clock (which is accurate to within one microsecond). The same seed will be used to generate a random number for all the sub-pixel positions of all the profiles. So in the former, the sub-pixel points checked for all the pixels undergoing Monte carlo integration in all profiles will be identical. In other words, the sub-pixel points in the first (closest to the center) pixel of all the profiles will be identical with each other. All the second pixels studied for all the profiles will also receive an identical (different from the first pixel) set of sub-pixel points and so on. As long as the number of random points used is large enough or the profiles are not identical, this should not cause any systematic bias. @node Oversampling, , Sampling from a function, Modeling basics @subsubsection Oversampling @cindex Oversampling The steps explained in @ref{Sampling from a function} do give an accurate representation of a profile prior to convolution. However, in an actual observation, the image is first convolved with or blurred by the atmospheric and instrument PSF in a continuous space and then it is sampled on the discrete pixels of the camera. @cindex PSF over-sample In order to more accurately simulate this process, the unconvolved image and the PSF are created on a finer pixel grid. In other words, the output image is a certain odd-integer multiple of the desired size, we can call this `oversampling'. The user can specify this multiple as a command-line option. The reason this has to be an odd number is that the PSF has to be centered on the center of its image. An image with an even number of pixels on each side does not have a central pixel. The image can then be convolved with the PSF (which should also be oversampled on the same scale). Finally, image can be sub-sampled to get to the initial desired pixel size of the output image. After this, mock noise can be added as explained in the next section. This is because unlike the PSF, the noise occurs in each output pixel, not on a continuous space like all the prior steps. @node If convolving afterwards, Flux Brightness and magnitude, Modeling basics, MakeProfiles @subsection If convolving afterwards In case you want to convolve the image later with a given point spread function, make sure to use a larger image size. After convolution, the profiles become larger and a profile that is normally completely outside of the image might fall within it. On one axis, if you want your final (convolved) image to be @mymath{m} pixels and your PSF is @mymath{2n+1} pixels wide, then when calling MakeProfiles, set the axis size to @mymath{m+2n}, not @mymath{m}. You also have to shift all the pixel positions of the profile centers on the that axis by @mymath{n} pixels to the positive. After convolution, you can crop the outer @mymath{n} pixels with the section crop box specification of ImageCrop: @option{--section=n:*-n,n:*-n} assuming your PSF is a square, see @ref{Crop section syntax}. This will also remove all discrete Fourier transform artifacts (blurred sides) from the final image. To facilitate this shift, MakeProfiles has the options @option{--xshift}, @option{--yshift} and @option{--prepforconv}, see @ref{Invoking astmkprof}. @node Flux Brightness and magnitude, Profile magnitude, If convolving afterwards, MakeProfiles @subsection Flux Brightness and magnitude @cindex ADU @cindex Gain @cindex Counts Astronomical data pixels are usually in units of counts@footnote{Counts are also known as analog to digital units (ADU).} or electrons or either one divided by seconds. To convert from the counts to electrons, you will need to know the instrument gain. In any case, they can be directly converted to energy or energy/time using the basic hardware (telescope, camera and filter) information. We will continue the discussion assuming the pixels are in units of energy/time. @cindex Flux @cindex Luminosity @cindex Brightness The @emph{brightness} of an object is defined as its total detected energy per time. This is simply the sum of the pixels that are associated with that detection by our detection tool for example @ref{NoiseChisel}@footnote{If further processing is done, for example the Kron or Petrosian radii are calculated, then the detected area is not sufficient and the total area that was within the respective radius must be used.}. The @emph{flux} of an object is in units of energy/time/area and for a detected object, it is defined as its brightness divided by the area used to collect the light from the source or the telescope aperture (for example in @mymath{cm^2})@footnote{For a full object that spans over several pixels, the telescope area should be used to find the flux. However, sometimes, only the brightness per pixel is desired. In such cases this book also @emph{loosely} uses the term flux. This is only approximately accurate however, since while all the pixels have a fixed area, the pixel size can vary with camera on the telescope.}. Knowing the flux (@mymath{f}) and distance to the object (@mymath{r}), we can calculate its @emph{luminosity}: @mymath{L=4{\pi}r^2f}. Therefore, flux and luminosity are intrinsic properties of the object, while brightness depends on our detecting tools (hardware and software). Here we will not be discussing luminosity, but brightness. However, since luminosity is the astrophysically interesting quantity, we also defined it here to avoid possible confusion between these two terms because they both have the same units. @cindex Magnitude zero-point @cindex Magnitudes from flux @cindex Flux to magnitude conversion @cindex Astronomical Magnitude system Images of astronomical objects span over a very large range of brightness. With the Sun (as the brightest object) being roughly @mymath{2.5^{60}=10^{24}} times brighter than the faintest galaxies we can currently detect. Therefore discussing brightness will be very hard, and astronomers have chosen to use a logarithmic scale to talk about the brightness of astronomical objects. But the logarithm can only be usable with a unit-less and always positive value. Fortunately brightness is always positive and to remove the units we divide the brightness of the object (@mymath{B}) by a reference brightness (@mymath{B_r}). We then define the resulting logarithmic scale as @mymath{magnitude} through the following relation@footnote{The @mymath{-2.5} factor in the definition of magnitudes is a legacy of the our ancient colleagues and in particular Hipparchus of Nicaea (190-120 BC).} @dispmath{m-m_r=-2.5\log_{10} \left( B \over B_r \right)} @cindex Zero-point magnitude @noindent @mymath{m} is defined as the magnitude of the object and @mymath{m_r} is the pre-defined magnitude of the reference brightness. One particularly easy condition is when @mymath{B_r=1}. This will allow us to summarize all the hardware specific parameters discussed above into one number as the reference magnitude which is commonly known as the Zero-point@footnote{When @mymath{B=Br=1}, the right side of the magnitude definition will be zero. Hence the name, ``zero-point''.} magnitude. @node Profile magnitude, Invoking astmkprof, Flux Brightness and magnitude, MakeProfiles @subsection Profile magnitude @cindex Brightness @cindex Truncation radius @cindex Sum for total flux To find the profile brightness or its magnitude, (see @ref{Flux Brightness and magnitude}), it is customary to use the 2D integration of the flux to infinity. However, in MakeProfiles we do not follow this idealistic approach and apply a more realistic method to find the total brightness or magnitude: the sum of all the pixels belonging to a profile within its predefined truncation radius. Note that if the truncation radius is not large enough, this can be significantly different from the total integrated light to infinity. @cindex Integration to infinity An integration to infinity is not a realistic condition because no galaxy extends indefinitely (important for high S@'ersic index profiles), pixelation can also cause a significant difference between the actual total pixel sum value of the profile and that of integration to infinity, especially in small and high S@'ersic index profiles. To be safe, you can specify a large enough truncation radius for such compact high S@'ersic index profiles. If oversampling is used then the brightness is calculated using the over-sampled image, see @ref{Oversampling} which is much more accurate. The profile is first built in an array completely bounding it with a normalization constant of unity (see @ref{Galaxies}). Taking @mymath{B} to be the desired brightness and @mymath{S} to be the sum of the pixels in the created profile, every pixel is then multiplied by @mymath{B/S} so the sum is exactly @mymath{B}. If the @option{--individual} option is called, this same array is written to a FITS file. If not, only the overlapping pixels of this array and the output image are kept and added to the output array. @node Invoking astmkprof, , Profile magnitude, MakeProfiles @subsection Invoking MakeProfiles MakeProfiles will make any number of profiles specified in a catalog either individually or in one image. The executable name is @file{astmkprof} with the following general template @example $ astmkprof [OPTION ...] [BackgroundImage] Catalog @end example @noindent One line examples: @example $ astmkprof background.fits catalog.txt $ astmkprof --xcol=0 --ycol=1 catalog.txt $ astmkprof --individual --oversample 3 -x500 -y500 catalog.txt @end example @noindent If mock images are to be made, the catalog (which stores the parameters for each mock profile) is the mandatory argument. The input catalog has to be a text file formatted in a table with columns separated by space, tab or comma (@key{,}) characters. See @ref{Common program behavior} for a complete explanation of some common behaviour and options in all Gnuastro programs including MakeProfiles. If a data image file (see @ref{Arguments}) is given, the pixels of that image are used as the background value for every pixel. The flux value of each profile pixel will be added to the pixel in that background value. In this case the values to all options relating to the output size and WCS will be ignored if specified (for example @option{--naxis1}, @option{--naxis2} and @option{--prepforconv}) on the command-line or in the configuration files. Note that @option{--oversample} will remain active even if a background image is specified. @menu * MakeProfiles catalog:: Required catalog properties. * MakeProfiles options:: Full list of MakeProfiles options. * MakeProfiles output:: The generated outputs. @end menu @node MakeProfiles catalog, MakeProfiles options, Invoking astmkprof, Invoking astmkprof @subsubsection MakeProfiles catalog The catalog is a text file table. Its columns can be ordered in any desired manner, you can specify which columns belong to which parameters using the set of options ending with @option{col}, for example @option{--xcol} or @option{--rcol}, see @ref{MakeProfiles options}. The value for the profile center in the catalog (in the @option{--xcol} and @option{--ycol} columns) can be a floating point number so the profile center can be on any sub-pixel position. Note that pixel positions in the FITS standard start from 1 and an integer is the pixel center. So a 2D image actually starts from the position (0.5, 0.5). In MakeProfiles profile centers do not have to be in the image. Even if only one pixel of the profile within the truncation radius is within the output image, that pixel is included in the image. Profiles that are completely out of the image will not be created. You can use the output log file to see which profiles were within the image. If PSF profiles (Moffat or Gaussian) are in the catalog and the profiles are to be built in one image (when @option{--individual} is not used), it is assumed they are the PSF(s) you want to convolve your created image with. So by default, they will not be built in the output image but as separate files. The sum of pixels of these separate files will also be set to unity (1) so you are ready to convolve, see @ref{Convolution process}. As a summary, their position and magnitude will be ignored. This behaviour can be disabled with the @option{--psfinimg} option. If you want to create all the profiles separately (with @option{--individual}) and you want the sum of the PSF profile pixels to be unity, you have to set their magnitudes in the catalog to the zero-point magnitude and be sure that the central positions of the profiles don't have any fractional part (the PSF center has to be in the center of the pixel). @node MakeProfiles options, MakeProfiles output, MakeProfiles catalog, Invoking astmkprof @subsubsection MakeProfiles options The common options that are shared by Gnuastro programs, are fully explained in @ref{Common options} and are not repeated here. Since there are no image inputs, the@option{--hdu} option is ignored. The options can be classified into the following categories: Output, Profiles, Catalog and WCS. Below each one is reviewed. @noindent Output: @table @option @item -x @itemx --naxis1 (@option{=INT}) The number of pixels in the output image along the first FITS axis (horizontal when viewed in SAO ds9). This is before over-sampling. For example if you call MakeProfiles with @option{--naxis1=100 --oversample=5} (assuming no shift due for later convolution), then the final image size along the first axis will be 500. If a background image is specified, any possible value to this option is ignored. @item -y @itemx --naxis2 (@option{=INT}) The number of pixels in the output image along the second FITS axis (vertical when viewed in SAO ds9), see the explanation for @option{--naxis1}. @item -T @itemx --type (@option{=STR}) Type of the output image pixels (specified by @code{BITPIX} in the FITS standard). It can have any one of the following values: @option{byte}, @option{short}, @option{long}, @option{longlong}, @option{float}, @option{double}. Internally, the images are made in the float type, but upon writing of the single output (not individual profiles), the image will be converted to the type specified by this option. When a background image is given without the @option{--inputascanvas} option, it is assumed that you want the output in the same format as the background, therefore the value to this option is ignored. @item -C @itemx --inputascanvas When an image is given as an argument, use the input image as the canvas to make all the mock profiles. In practice, this option only changes the non-blank pixels (see @ref{Blank pixels}) of the input image (in memory after reading, not the actual input file) to zero before making the profiles. The profiles are then built on those cleared pixels. With this option (like when building on a background image) the values to @option{--naxis1}, @option{--naxis2}, @option{--crpix1}, @option{--crpix2}, @option{--crval1}, @option{--crval2}, and @option{--resolution} are ignored. However, if @option{--type} is given, its value will take precedence over the background image type. This option can be very useful when the mock image is to be made over a real sky region and compared to a real image (that might have blank pixels. One example can be when you want to make circular or elliptical labeled regions to feed into MakeCatalog along with NoiseChisel's outputs for aperture photometry. See the discussion and examples under the `@option{--mforflatpix}' for more. @item -s @itemx --oversample (@option{=INT}) The scale to over-sample the profiles and final image. If not an odd number, will be added by one, see @ref{Oversampling}. Note that this @option{--oversample} will remain active even if an input image is specified. If your input catalog is based on the background image, be sure to set @option{--oversample=1}. @item --psfinimg Build the possibly existing PSF profiles (Moffat or Gaussian) in the catalog into the final image. By default they are built separately so you can convolve your images with them, thus their magnitude and positions are ignored. With this option, they will be built in the final image like every other galaxy profile. To have a final PSF in your image, make a point profile where you want the PSF and after convolution it will be the PSF. @item -i @itemx --individual @cindex Individual profiles @cindex Build individual profiles If this option is called, each profile is created in a separate FITS file within the same directory as the output and the row number of the profile (starting from zero) in the name. The file for each row's profile will be in the same directory as the final combined image of all the profiles and will have the final image's name as a suffix. So for example if the final combined image is named @file{./out/fromcatalog.fits}, then the first profile that will be created with this option will be named @file{./out/0_fromcatalog.fits}. Since each image only has one full profile out to the truncation radius the profile is centered and so, only the sub-pixel position of the profile center is important for the outputs of this option. The output will have an odd number of pixels. If there is no oversampling, the central pixel will contain the profile center. If the value to @option{--oversample} is larger than unity, then the profile center is on any of the central @option{--oversample}'d pixels depending on the fractional value of the profile center. If the fractional value is larger than half, it is on the bottom half of the central region. This is due to the FITS definition of a real number position: The center of a pixel has fractional value @mymath{0.00} so each pixel contains these fractions: .5 -- .75 -- .00 (pixel center) -- .25 -- .5. @item -m @itemx --nomerged Don't make a merged image. By default after making the profiles, they are added to a final image with sides of @option{--naxis1} and @option{--naxis2} if they overlap with it. @end table @noindent Profiles: @table @option @item -r @itemx --numrandom The number of random points used in the central regions of the profile, see @ref{Sampling from a function}. @item -e @itemx --envseed Use the value to the @code{GSL_RNG_SEED} environment variable to generate the random Monte Carlo sampling distribution, see @ref{Sampling from a function} and @ref{Generating random numbers}. @item -t @itemx --tolerance (@option{=FLT}) The tolerance to switch from Monte Carlo integration to the central pixel value, see @ref{Sampling from a function}. @item -p @itemx --tunitinp The truncation column of the catalog is in units of pixels. By default, the truncation column is considered to be in units of the radial parameters of the profile (@option{--rcol}). Read it as `t-unit-in-p' for `truncation unit in pixels'. @item -X @itemx --xshift (@option{=INT}) Shift all the profiles and enlarge the image along the first FITS axis, see @mymath{n} in @ref{If convolving afterwards}. This is useful when you want to convolve the image afterwards. If you are using an external PSF, be sure to oversample it to the same scale used for creating the mock images. If a background image is specified, any possible value to this option is ignored. @item -Y @itemx --yshift (@option{=INT}) Similar to @option{--xshift} for the second FITS axis. @item -c @itemx --prepforconv Shift all the profiles and enlarge the image based on half the width of the first Moffat or Gaussian profile in the catalog, considering any possible oversampling see @ref{If convolving afterwards}. @option{--prepforconv} is only checked and possibly activated if @option{--xshift} and @option{--yshift} are both zero (after reading the command-line and configuration files). If a background image is specified, any possible value to this option is ignored. @item --magatpeak The magnitude column in the catalog (see @ref{MakeProfiles catalog}) will be used to find the brightness only for the peak profile pixel, not the full profile. Note that this is the flux of the profile's peak pixel in the final output of MakeProfiles. So beware of the oversampling, see @ref{Oversampling}. This option can be useful if you want to check a mock profile's total magnitude at various truncation radii. Without this option, no matter what the truncation radius is, the total magnitude will be the same as that given in the catalog. But with this option, the total magnitude will become brighter as you increase the truncation radius. In sharper profiles, sometimes the accuracy of measuring the peak profile flux is more than the overall object brightness. In such cases, with this option, the final profile will be built such that its peak has the given magnitude, not the total profile. @cartouche @strong{CAUTION:} If you want to use this option for comparing with observations, please note that MakeProfiles does not do convolution. Unless you have de-convolved your data, your images are convolved with the instrument and atmospheric PSF, see @ref{PSF}. Particularly in sharper profiles, the flux in the peak pixel is strongly decreased after convolution. Also note that in such cases, besides de-convolution, you will have to set @option{--oversample=1} otherwise after resampling your profile with ImageWarp (see @ref{ImageWarp}), the peak flux will be different. @end cartouche @item -R @itemx --replace Do not add the pixels of each profile over the background (possibly crowded by other profiles), replace them. By default, when two profiles overlap, the final pixel value is the sum of all the profiles that overlap on that pixel. When this option is given, the pixels are not added but replaced by the newer profile's pixel and any value under it is lost. @cindex CPU threads @cindex Threads, CPU When order matters, make sure to use this function with `@option{--numthreads=1}'. When multiple threads are used, the separate profiles are built asynchronously and not in order. Since order does not matter in an addition, this causes no problems by default but has to be considered when this option is given. Using multiple threads is no problem if the profiles are to be used as a mask with a blank or fixed value (see `@option{--mforflatpix}') since all their pixel values are the same. Note that only non-zero pixels are replaced. With radial profiles (for example S@'ersic or Moffat) only values above zero will be part of the profile. However, when using flat profiles with the `@option{--mforflatpix}' option, you should be careful not to give a @code{0.0} value as the flat profile's pixel value. @item -w @itemx --circumwidth (@option{=FLT}) The width of the circumference if the profile is to be an elliptical circumference or annulus. See the explanations for this type of profile in @option{--fcol}. @item -z @itemx --zeropoint (@option{=FLT}) The zero-point magnitude of the image. @end table @noindent Catalog: The value to all of these options is considered to be a column number, where counting starts from zero. @table @option @item --fcol (@option{=INT}) The functional form of the profile with one of the values below. Note that this value will be converted to an integer before analysis using the internal type conversion of C. So for example 2.80 will be converted to 2. @itemize @item 0: S@'ersic. @item 1: Moffat. @item 2: Gaussian. @item 3: Point source (a star). @item 4: Flat profile: all pixels have same value. @item 5: Circumference: same value for all pixels between the truncation radius (@mymath{r_t}) and @mymath{r_t-w} where @mymath{w} is the value to the @option{--circumwidth}. Currently this is only intended to be used for making an elliptical annulus (with a width of 1 or 2 pixels). @end itemize @item --xcol (@option{=INT}) The center of the profiles along the first FITS axis (horizontal when viewed in SAO ds9). See the explanations for @option{--racol} for precedence when both image and WCS coordinate columns are given. @item --ycol (@option{=INT}) The center of the profiles along the second FITS axis (vertical when viewed in SAO ds9). Similar to @option{--xcol}. @item --racol (@option{=INT}) The profile center's right ascension. Along with @option{--deccol}, these WCS coordinate columns are not mandatory. If they are not given, the @option{--xcol} and @option{--ycol} options will be used to specify the profile's central position and vice-versa. However, if image coordinate columns (@option{--xcol} and @option{--ycol}) and WCS coordinate columns (@option{--racol} and @option{--deccol}) are given, the WCS coordinate columns take precedence and image coordinate columns will be ignored. @item --deccol (@option{=INT}) The profile center's declination. Similar to @option{--racol}. @item --rcol (@option{=INT}) The radius parameter of the profiles. Effective radius (@mymath{r_e}) if S@'ersic, FWHM if Moffat or Gaussian. @item --ncol (@option{=INT}) The S@'ersic index (@mymath{n}) or Moffat @mymath{\beta}. @item --pcol (@option{=INT}) The position angle (in degrees) of the profiles relative to the first FITS axis (horizontal when viewed in SAO ds9). @item --qcol (@option{=INT}) The axis ratio of the profiles (minor axis divided by the major axis). @item --mcol (@option{=INT}) The total pixelated magnitude of the profile within the truncation radius, see @ref{Profile magnitude}. @item --tcol (@option{=INT}) The truncation radius of this profile. By default it is in units of the radial parameter of the profile (the value in the @option{--rcol} of the catalog). If @option{--tunitinp} is given, this value is interpreted in units of pixels (prior to oversampling) irrespective of the profile. @item -F @itemx --mforflatpix When making fixed value profiles (flat and circumference, see `@option{--fcol}'), don't use the value in the column specified by `@option{--mcol}' as the magnitude. Instead use it as the exact value that all the pixels of these profiles should have. This option is irrelevant for other types of profiles. This option is very useful for creating masks, or labeled regions in an image. Any integer, or floating point value can used in this column with this option, including @code{NaN} (or `@code{nan}', or `@code{NAN}', case is irrelevant), and infinities (@code{inf}, @code{-inf}, or @code{+inf}). For example, with this option if you set the value in the magnitude column (@option{--mcol}) to @code{NaN}, you can create an elliptical or circular mask over an image (which can be given as the argument), see @ref{Blank pixels}. Another useful application of this option is to create labeled elliptical or circular apertures in an image. To do this, set the value in the magnitude column to the label you want for this profile. This labeled image can then be used in combination with NoiseChisel's output (see @ref{NoiseChisel output}) to do aperture photometry with MakeCatalog (see @ref{MakeCatalog}). Alternatively, if you want to mark regions of the image (for example with an elliptical circumference) and you don't want to use NaN values (as explained above) for some technical reason, you can get the minimum or maximum value in the image @footnote{The minimum will give a better result, because the maximum can be too high compared to most pixels in the image, making it harder to display.} using Arithmetic (see @ref{Arithmetic}), then use that value in the magnitude column along with this option for all the profiles. Please note that when using MakeProfiles on an already existing image, you have to set `@option{--oversample=1}'. Otherwise all the profiles will be scaled up based on the oversampling scale in your configuration files (see @ref{Configuration files}) unless you have accounted for oversampling in your catalog. @end table @noindent WCS: @table @option @item --crpix1 (@option{=FLT}) The pixel coordinates of the WCS reference point on the first (horizontal) FITS axis (counting from 1). @item --crpix2 (@option{=FLT}) The pixel coordinates of the WCS reference point on the second (vertical) FITS axis (counting from 1). @item --crval1 (@option{=FLT}) The Right Ascension (RA) of the reference point. @item --crval2 (@option{=FLT}) The Declination of the reference point. @item --resolution (@option{=FLT}) The resolution of the non-oversampled image in units of arcseconds/pixel. @end table @node MakeProfiles output, , MakeProfiles options, Invoking astmkprof @subsubsection MakeProfiles output Besides the final merged image of all the profiles or individual profiles that can be built based on the input options, MakeProfiles will also create a log file in the current directory (where you run MockProfiles). The values for each column are explained in the first few commented (starting with @command{#} character). The log file includes the following information: @itemize @item The total magnitude of the profile in the image. This will be different from your input magnitude if the profile was not completely in the image. @item The number of pixels (in the oversampled image) which used Monte Carlo integration and not the central pixel value. @item The fraction of flux in the Monte Carlo integrated pixels. @item If an individual image was created or not. @end itemize @node MakeNoise, , MakeProfiles, Modeling and fittings @section MakeNoise @cindex Noise Real data are always buried in noise, therefore to finalize a simulation of real data (for example to test our observational algorithms) it is essential to add noise to the mock profiles created with MakeProfiles, see @ref{MakeProfiles}. Below, the general principles and concepts to help understand how noise is quantified is discussed. MakeNoise options and argument are then discussed in @ref{Invoking astmknoise}. @menu * Noise basics:: Noise concepts and definitions. * Invoking astmknoise:: Options and arguments to MakeNoise. @end menu @node Noise basics, Invoking astmknoise, MakeNoise, MakeNoise @subsection Noise basics @cindex Noise @cindex Image noise Deep astronomical images, like those used in extragalactic studies seriously suffer from noise in the data. Generally speaking, the sources of noise in an astronomical image are photon counting noise and Instrumental noise which are discussed in detail below. We finish with a short introduction on how random numbers are generated and how you can determine the random number generator and seed value. @menu * Photon counting noise:: Poisson noise * Instrumental noise:: Readout, dark current and other sources. * Final noised pixel value:: How the final noised value is calculated. * Generating random numbers:: How random numbers are generated. @end menu @node Photon counting noise, Instrumental noise, Noise basics, Noise basics @subsubsection Photon counting noise @cindex Counting error @cindex Photon counting noise Thanks to the very accurate electronics used in today's detectors, this type of noise is the main cause of concern for extra galactic studies. It can generally be associate with the counting error that is known to have a Poisson distribution. The Poisson distribution is about counting. But counting is a discrete operation with only positive values, for example we can't count @mymath{3.2} or @mymath{-2} of anything. We only count @mymath{0}, @mymath{1}, @mymath{2}, @mymath{3} and so on. Therefore the Poisson distribution is also a discrete distribution, only applying to whole positive integers. Let's assume the mean value of counting something is known. In this case, the number of electrons that are produced by photons in the CCD. Let's call this mean @mymath{\lambda}. Let's take @mymath{k} to represent the result of counting in one particular time we attempt to count. The probability density function of @mymath{k} can be written as: @cindex Poisson distribution @dispmath{f(k)={\lambda^k \over k!} e^{-\lambda},\quad k\in @{0, 1, 2, 3, \dots @}} @cindex Skewed Poisson distribution Because the Poisson distribution is only applicable to positive values, it is by nature very skewed when @mymath{\lambda} is near zero. One qualitative way to imagine it is that there simply aren't enough integers smaller than @mymath{\lambda}, than there are larger integers. Therefore to accommodate all possibilities, it has to be skewed when @mymath{\lambda} is small. @cindex Compare Poisson and Gaussian But as @mymath{\lambda} becomes larger and larger, the distribution becomes more and more symmetric. One very useful property of the Poisson distribution is that the mean value is also its variance. When @mymath{\lambda} is very large, say @mymath{\lambda>1000}, then the normal (Gaussian) distribution, see @ref{PSF}, is an excellent approximation of the Poisson distribution with mean @mymath{\mu=\lambda} and standard deviation @mymath{\sigma=\sqrt{\lambda}}. We see that the variance or dispersion of the distribution depends on the mean value, and when it is large it can be approximated with a Gaussian that only has one free parameter (@mymath{\mu=\lambda} and @mymath{\sigma=\sqrt{\lambda}}) instead of two that it originally has. @cindex Sky value @cindex Background flux @cindex Undetected objects The astronomical objects after convolution with the PSF of the instrument, lie above a certain background flux. This background flux is defined to be the average flux of a region in the image that has absolutely no objects. The physical origin of this background value is the brightness of the atmosphere or possible stray light within the imaging instrument. It is thus an ideal definition, because in practice, what lies deep in the noise far lower than the detection limit is never known@footnote{See the section on sky in Akhlaghi M., Ichikawa. T. 2015. Astrophysical Journal Supplement Series.}. However, in a real image, a relatively large number of very faint objects can been fully buried in the noise. These undetected objects will bias the background measurement to slightly larger values. The sky value is therefore defined to be the average of the undetected regions in the image, so in an ideal case where all the objects have been detected, the sky value and background value are the same. @cindex Background flux gradients @cindex Gradients in background flux @cindex Variation of background flux As longer wavelengths are used, the background value becomes more significant and also varies over a wide image field. Such variations are not currently implemented in MakeProfiles, but will be in the future. In a mock image, we have the luxury of setting the background value. @cindex Simulating noise @cindex Noise simulation In each pixel of the canvas of pixels, the flux is the sum of contributions from various sources after convolution. Let's name this flux of the convolved sum of possibly overlapping objects, @mymath{I_{nn}}. @mymath{nn} representing `no noise'. For now, let's assume the background is constant and represented by @mymath{B}. In practice the background values are larger than @mymath{\sim1,000} counts. Then the flux after adding noise is a random value taken from a Gaussian distribution with the following mean (@mymath{\mu}) and standard deviation (@mymath{\sigma}): @dispmath{\mu=B+I_{nn}, \quad \sigma=\sqrt{B+I_{nn}}} Since this type of noise is inherent in the objects we study, it is usually measured on the same scale as the astronomical objects, namely the magnitude system, see @ref{Flux Brightness and magnitude}. It is then internally converted to the flux scale for further processing. @node Instrumental noise, Final noised pixel value, Photon counting noise, Noise basics @subsubsection Instrumental noise @cindex Readout noise @cindex Instrumental noise @cindex Noise, instrumental While taking images with a camera, a dark current is fed to the pixels, the variation of the value of this dark current over the pixels, also adds to the final image noise. Another source of noise is the readout noise that is produced by the electronics in the CCD that attempt to digitize the voltage produced by the photo-electrons in the analog to digital converter. In deep extra-galactic studies these sources of noise are not as significant as the noise of the background sky. Let @mymath{C} represent the combined standard deviation of all these sources of noise. If only this source of noise is present, the noised pixel value would be a random value chosen from a Gaussian distribution with @dispmath{\mu=I_{nn}, \quad \sigma=\sqrt{C^2+I_{nn}}} @cindex ADU @cindex Gain @cindex Counts This type of noise is completely independent of the type of objects being studied, it is completely determined by the instrument. So the flux scale (and not magnitude scale) is most commonly used for this type of noise. In practice, this value is usually reported in ADUs not flux or electron counts. The gain value of the device can be used to convert between these two, see @ref{Flux Brightness and magnitude}. @node Final noised pixel value, Generating random numbers, Instrumental noise, Noise basics @subsubsection Final noised pixel value Depending on the values you specify for @mymath{B} and @mymath{C} from the above, the final noised value for each pixel is a random value chosen from a Gaussian distribution with @dispmath{\mu=B+I_{nn}, \quad \sigma=\sqrt{C^2+B+I_{nn}}} @node Generating random numbers, , Final noised pixel value, Noise basics @subsubsection Generating random numbers @cindex Random numbers @cindex Numbers, random As discussed above, to generate noise we need to make random samples of a particular distribution. So it is important to understand some general concepts regarding the generation of random numbers. For a very complete and nice introduction we strongly advise reading Donald Knuth's ``The art of computer programming'', volume 2, chapter 3@footnote{Knuth, Donald. 1998. The art of computer programming. Addison--Wesley. ISBN 0-201-89684-2 }. Quoting from the GNU Scientific Library manual, ``If you don't own it, you should stop reading right now, run to the nearest bookstore, and buy it''@footnote{For students, running to the library might be more affordable!}! @cindex Psudo-random numbers @cindex Numbers, psudo-random @cindex Seed, psudo-random numbers Using only software, we can only produce what is called a psudo-random sequence of numbers. A true random number generator is a hardware (let's assume we have made sure it has no systematic biases), for example throwing dice or flipping coins (which have remained from the ancient times). More modern hardware methods use atmospheric noise, thermal noise or other types of external electromagnetic or quantum phenomena. All psudo-random number generators (software) require a seed to be the basis of the generation. The advantage of having a seed is that if you specify the same seed for multiple runs, you will get an identical sequence of random numbers which allows you to reproduce the same final noised image. @cindex Environment variables @cindex GNU Scientific Library The programs in GNU Astronomy Utilities (for example MakeNoise or MakeProfiles) use the GNU Scientific Library (GSL) to generate random numbers. GSL allows the user to set the random number generator through environment variables, see @ref{Installation directory} for an introduction to environment variables. In the chapter titled ``Random Number Generation'' they have fully explained the various random number generators that are available (there are a lot of them!). Through the two environment variables @code{GSL_RNG_TYPE} and @code{GSL_RNG_SEED} you can specify the generator and its seed respectively. If you don't specify a value for @code{GSL_RNG_TYPE}, GSL will use its default random number generator type. The default type is sufficient for most general applications. If no value is given for the @code{GSL_RNG_SEED} environment variable and you have asked Gnuastro to read the seed from the environment (through the @option{--envseed} option), then GSL will use the default value of each generator to give identical outputs. If you don't explicitly tell Gnuastro programs to read the seed value from the environment variable, then they will use the system time (accurate to within a microsecond) to generate (apparently random) seeds. In this manner, every time you run the program, you will get a different random number distribution. There are two ways you can specify values for these environment variables. You can call them on the same command-line for example: @example $ GSL_RNG_TYPE="taus" GSL_RNG_SEED=345 astmknoise input.fits @end example @noindent In this manner the values will only be used for this particular execution of MakeNoise. To define them for the full period of your terminal session or script length, you can use the shell's @command{export} command (for a script remove the @code{$} signs): @example $ export GSL_RNG_TYPE="taus" $ export GSL_RNG_SEED=345 @end example @cindex Startup scripts @cindex @file{.bashrc} @noindent The subsequent programs which use GSL's random number generators will hence forth use these values in this session of the terminal you are running or while executing this script. In case you want set fixed values for these variables every time you use the GSL random number generator, you can add these two lines to your @file{.bashrc} startup script@footnote{Don't forget that if you are going to give your scripts (that use the GSL random number generator) to others you have to make sure you also tell them to set these environment variable separately. So for scripts, it is best to keep all such variable definitions within the script, even if they are within your @file{.bashrc}.}, see @ref{Installation directory}. @cartouche @noindent @strong{NOTE:} If the two environment variables @code{GSL_RNG_TYPE} and @code{GSL_RNG_SEED} are defined, GSL will report them by default, even if you don't use the @option{--envseed} option. For example you can see the top few lines of the output of MakeProfiles: @example $ export GSL_RNG_TYPE="taus" $ export GSL_RNG_SEED=345 $ astmkprof catalog.txt --envseed GSL_RNG_TYPE=taus GSL_RNG_SEED=345 MakeProfiles started on AAA BBB DD EE:FF:GG HHH - 6 profiles read from catalog.txt 0.000236 seconds - Random number generator (RNG) type: taus - RNG seed for all profiles: 345 @end example @noindent The first two output lines (showing the names of the environment variables) are printed by GSL before MakeProfiles actually starts generating random numbers. The Gnuastro programs will report the values they use independently, you should check them for the final values used. For example if @option{--envseed} is not given, @code{GSL_RNG_SEED} will not be used and the last line shown above will not be printed. In the case of MakeProfiles, each profile will get its own seed value. @end cartouche @node Invoking astmknoise, , Noise basics, MakeNoise @subsection Invoking MakeNoise MakeNoise will add noise to an existing image. The executable name is @file{astmknoise} with the following general template @example $ astmknoise [OPTION ...] InputImage.fits @end example @noindent One line examples: @example $ astmknoise --background=1000 --stdadd=20 mockimage.fits @end example @noindent If actual processing is to be done, the input image is a mandatory argument. The full list of options common to all the programs in Gnuastro can be seen in @ref{Common options}. The output will have the same type as the input image, however the internal processing is done on a double precision floating point format. If the input values were integer types, then each floating point number will be rounded to the nearest integer away from zero. This might cause integer overflow if types with small ranges are used (for example images with a @code{BITPIX} of @code{8} which can only keep 256 values). This can be disabled with the @option{doubletype} option. The header of the output FITS file keeps all the parameters that were influential in making it. This is done for future reproducibility. @table @option @item -b @itemx --background (@option{=FLT}) The background pixel value for the image in units of magnitudes, see @ref{Photon counting noise} and @ref{Flux Brightness and magnitude}. @item -z @itemx --zeropoint (@option{=FLT}) The zeropoint magnitude used to convert the value of @option{--background} (in units of magnitude) to flux, see @ref{Flux Brightness and magnitude}. @item -s @itemx --stdadd (@option{=FLT}) The instrumental noise which is in units of flux, see @ref{Instrumental noise}. @item -e @itemx --envseed Use the @code{GSL_RNG_SEED} environment variable for the seed used in the random number generator, see @ref{Generating random numbers}. With this option, the output image noise is always going to be identical (or reproducible). @item -d @itemx --doubletype Save the output in the double precision floating point format that was used internally. This option will be most useful if the input images were of integer types. @end table @c @node Table manipulation, High-level calculations, Modeling and fittings, Top @c @chapter Table manipulation @c @c @cindex Table manipulation @c @cindex Manipulating tables @c The FITS standard also specifies tables as a form of data that can be @c stored in the extensions of a FITS file. These tables can be ASCII @c tables or binary tables. The programs in this section provide the @c tools to directly read and write to FITS tables. @c @c The software for this section have to be added .... @node High-level calculations, Libraries, Modeling and fittings, Top @chapter High-level calculations After the reduction of raw data (for example with the programs in @ref{Image manipulation}) you will have reduced images/data ready for processing/analyzing (for example with the programs in @ref{Image analysis}). But the processed/analyzed data (or catalogs) are still not enough to derive any scientific result. Even higher-level analysis is still needed to convert the observed magnitudes, sizes or volumes into physical quantities that we associate with each catalog entry or detected object which is the purpose of the tools in this section. @menu * CosmicCalculator:: Calculate cosmological variables @end menu @node CosmicCalculator, , High-level calculations, High-level calculations @section CosmicCalculator To derive higher-level information regarding our sources in extra-galactic astronomy, cosmological calculations are necessary. In Gnuastro, CosmicCalculator is in charge of such calculations. Before discussing how CosmicCalculator is called and operates (in @ref{Invoking astcosmiccal}), it is important to provide a rough but mostly self sufficient review of the basics and the equations used in the analysis. In @ref{Distance on a 2D curved space} the basic idea of understanding distances in a curved and expanding 2D universe (which we can visualize) are reviewed. Having solidified the concepts there, in @ref{Extending distance concepts to 3D}, the formalism is extended to the 3D universe we are trying to study in our research. The focus here is obtaining a physical insight into these equations (mainly for the use in real observational studies). There are many books thoroughly deriving and proving all the equations with all possible initial conditions and assumptions for any abstract universe, interested readers can study those books. @menu * Distance on a 2D curved space:: Distances in 2D for simplicity * Extending distance concepts to 3D:: Going to 3D (our real universe). * Invoking astcosmiccal:: How to run CosmicCalculator @end menu @node Distance on a 2D curved space, Extending distance concepts to 3D, CosmicCalculator, CosmicCalculator @subsection Distance on a 2D curved space The observations to date (for example the Plank 2013 results), have not measured the presence of a significant curvature in the universe. However to be generic (and allow its measurement if it does in fact exist), it is very important to create a framework that allows curvature. As 3D beings, it is impossible for us to mentally create (visualize) a picture of the curvature of a 3D volume in a 4D space. Hence, here we will assume a 2D surface and discuss distances on that 2D surface when it is flat, or when the 2D surface is curved (in a 3D space). Once the concepts have been created/visualized here, in @ref{Extending distance concepts to 3D}, we will extend them to the real 3D universe we live in and hope to study. To be more understandable (actively discuss from an observer's point of view) let's assume we have an imaginary 2D friend living on the 2D space (which @emph{might} be curved in 3D). So here we will be working with it in its efforts to analyze distances on its 2D universe. The start of the analysis might seem too mundane, but since it is impossible to imagine a 3D curved space, it is important to review all the very basic concepts thoroughly for an easy transition to a universe we cannot visualize any more (a curved 3D space in 4D). To start, let's assume a static (not expanding or shrinking), flat 2D surface similar to @ref{flatplane} and that our 2D friend is observing its universe from point @mymath{A}. One of the most basic ways to parametrize this space is through the Cartesian coordinates (@mymath{x}, @mymath{y}). In @ref{flatplane}, the basic axes of these two coordinates are plotted. An infinitesimal change in the direction of each axis is written as @mymath{dx} and @mymath{dy}. For each point, the infinitesimal changes are parallel with the respective axes and are not shown for clarity. Another very useful way of parametrizing this space is through polar coordinates. For each point, we define a radius (@mymath{r}) and angle (@mymath{\phi}) from a fixed (but arbitrary) reference axis. In @ref{flatplane} the infinitesimal changes for each polar coordinate are plotted for a random point and a dashed circle is shown for all points with the same radius. @float Figure,flatplane @center@image{gnuastro-figures/flatplane, 10cm, , } @caption{Two dimensional Cartesian and polar coordinates on a flat plane.} @end float Assuming a certain position, which can be parametrized as @mymath{(x,y)}, or @mymath{(r,\phi)}, a general infinitesimal change change in its position will place it in the coordinates @mymath{(x+dx,y+dy)} and @mymath{(r+dr,\phi+d\phi)}. The distance (on the flat 2D surface) that is covered by this infinitesimal change in the static universe (@mymath{ds_s}, the subscript signifies the static nature of this universe) can be written as @dispmath{ds_s=dx^2+dy^2=dr^2+r^2d\phi^2}The main question is this: how can our 2D friend incorporate the (possible) curvature in its universe when it is calculating distances? The universe it lives in might equally be a locally flat but globally curved surface like @ref{sphericalplane}. The answer to this question but for a 3D being (us) is the whole purpose to this discussion. So here we want to give our 2D friend (and later, ourselves) the tools to measure distances if the space (that hosts the objects) is curved. @ref{sphericalplane} assumes a spherical shell with radius @mymath{R} as the curved 2D plane for simplicity. The spherical shell is tangent to the 2D plane and only touches it at @mymath{A}. The result will be generalized afterwards. The first step in measuring the distance in a curved space is to imagine a third dimension along the @mymath{z} axis as shown in @ref{sphericalplane}. For simplicity, the @mymath{z} axis is assumed to pass through the center of the spherical shell. Our imaginary 2D friend cannot visualize the third dimension or a curved 2D surface within it, so the remainder of this discussion is purely abstract for it (similar to us being unable to visualize a 3D curved space in 4D). But since we are 3D creatures, we have the advantage of visualizing the following steps. Fortunately our 2D friend knows our mathematics, so it can follow along with us. With the third axis added, a generic infinitesimal change over @emph{the full} 3D space corresponds to the distance: @dispmath{ds_s^2=dx^2+dy^2+dz^2=dr^2+r^2d\phi^2+dz^2.}It is very important to recognize that this change of distance is for @emph{any} point in the 3D space, not just those changes that occur on the 2D spherical shell of @ref{sphericalplane}. Recall that our 2D friend can only do measurements in the 2D spherical shell, not the full 3D space. So we have to constrain this general change to any change on the 2D spherical shell. To do that, let's look at the arbitrary point @mymath{P} on the 2D spherical shell. Its image (@mymath{P'}) on the flat plain is also displayed. From the dark triangle, we see that @float Figure,sphericalplane @center@image{gnuastro-figures/sphericalplane, 10cm, , } @caption{2D spherical plane (centered on @mymath{O}) and flat plane (gray) tangent to it at point @mymath{A}.} @end float @dispmath{\sin\theta={r\over R},\quad\cos\theta={R-z\over R}.}These relations allow our 2D friend to find the value of @mymath{z} (an abstract dimension for it) as a function of r (distance on a flat 2D plane, which it can visualize) and thus eliminate @mymath{z}. From @mymath{\sin^2\theta+\cos^2\theta=1}, we get @mymath{z^2-2Rz+r^2=0} and solving for @mymath{z}, we find: @dispmath{z=R\left(1\pm\sqrt{1-{r^2\over R^2}}\right).}The @mymath{\pm} can be understood from @ref{sphericalplane}: For each @mymath{r}, there are two points on the sphere, one in the upper hemisphere and one in the lower hemisphere. An infinitesimal change in @mymath{r}, will create the following infinitesimal change in @mymath{z}: @dispmath{dz={\mp r\over R}\left(1\over \sqrt{1-{r^2/R^2}}\right)dr.}Using the positive signed equation instead of @mymath{dz} in the @mymath{ds_s^2} equation above, we get: @dispmath{ds_s^2={dr^2\over 1-r^2/R^2}+r^2d\phi^2.} The derivation above was done for a spherical shell of radius @mymath{R} as a curved 2D surface. To generalize it to any surface, we can define @mymath{K=1/R^2} as the curvature parameter. Then the general infinitesimal change in a static universe can be written as: @dispmath{ds_s^2={dr^2\over 1-Kr^2}+r^2d\phi^2.}Therefore, we see that a positive @mymath{K} represents a real @mymath{R} which signifies a closed 2D spherical shell like @ref{sphericalplane}. When @mymath{K=0}, we have a flat plane (@ref{flatplane}) and a negative @mymath{K} will correspond to an imaginary @mymath{R}. The latter two cases are open universes (where @mymath{r} can extend to infinity). However, when @mymath{K>0}, we have a closed universe, where @mymath{r} cannot become larger than @mymath{R} as in @ref{sphericalplane}. @cindex Proper distance A very important issue that can be discussed now (while we are still in 2D and can actually visualize things) is that @mymath{\overrightarrow{r}} is tangent to the curved space at the observer's position. In other words, it is on the gray flat surface of @ref{sphericalplane}, even when the universe if curved: @mymath{\overrightarrow{r}=P'-A}. Therefore for the point @mymath{P} on a curved space, the raw coordinate @mymath{r} is the distance to @mymath{P'}, not @mymath{P}. The distance to the point @mymath{P} (at a specific coordinate @mymath{r} on the flat plane) on the curved surface (thick line in @ref{sphericalplane}) is called the @emph{proper distance} and is displayed with @mymath{l}. For the specific example of @ref{sphericalplane}, the proper distance can be calculated with: @mymath{l=R\theta} (@mymath{\theta} is in radians). using the @mymath{\sin\theta} relation found above, we can find @mymath{l} as a function of @mymath{r}: @dispmath{\theta=\sin^{-1}\left({r\over R}\right)\quad\rightarrow\quad l(r)=R\sin^{-1}\left({r\over R}\right)}@mymath{R} is just an arbitrary constant and can be directly found from @mymath{K}, so for cleaner equations, it is common practice to set @mymath{R=1}, which gives: @mymath{l(r)=\sin^{-1}r}. Also note that if @mymath{R=1}, then @mymath{l=\theta}. Generally, depending on the the curvature, in a @emph{static} universe the proper distance can be written as a function of the coordinate @mymath{r} as (from now on we are assuming @mymath{R=1}): @dispmath{l(r)=\sin^{-1}(r)\quad(K>0),\quad\quad l(r)=r\quad(K=0),\quad\quad l(r)=\sinh^{-1}(r)\quad(K<0).}With @mymath{l}, the infinitesimal change of distance can be written in a more simpler and abstract form of @dispmath{ds_s^2=dl^2+r^2d\phi^2.} @cindex Comoving distance Until now, we had assumed a static universe (not changing with time). But our observations so far appear to indicate that the universe is expanding (isn't static). Since there is no reason to expect the observed expansion is unique to our particular position of the universe, we expect the universe to be expanding at all points with the same rate at the same time. Therefore, to add a time dependence to our distance measurements, we can simply add a multiplicative scaling factor, which is a function of time: @mymath{a(t)}. The functional form of @mymath{a(t)} comes from the cosmology and the physics we assume for it: general relativity. With this scaling factor, the proper distance will also depend on time. As the universe expands (moves), the distance will also move to larger values. We thus define a distance measure, or coordinate, that is independent of time and thus doesn't `move' which we call the @emph{comoving distance} and display with @mymath{\chi} such that: @mymath{l(r,t)=\chi(r)a(t)}. We thus shift the @mymath{r} dependence of the proper distance we derived above for a static universe to the comoving distance: @dispmath{\chi(r)=\sin^{-1}(r)\quad(K>0),\quad\quad \chi(r)=r\quad(K=0),\quad\quad \chi(r)=\sinh^{-1}(r)\quad(K<0).} Therefore @mymath{\chi(r)} is the proper distance of an object at a specific reference time: @mymath{t=t_r} (the @mymath{r} subscript signifies ``reference'') when @mymath{a(t_r)=1}. At any arbitrary moment (@mymath{t\neq{t_r}}) before or after @mymath{t_r}, the proper distance to the object can simply be scaled with @mymath{a(t)}. Measuring the change of distance in a time-dependent (expanding) universe will also involve the speed of the object changing positions. Hence, let's assume that we are only thinking about the change in distance caused by something (light) moving at the speed of light. This speed is postulated as the only constant and frame-of-reference-independent speed in the universe, making our calculations easier, light is also the major source of information we receive from the universe, so this is a reasonable assumption for most extra-galactic studies. We can thus parametrize the change in distance as @dispmath{ds^2=c^2dt^2-a^2(t)ds_s^2 = c^2dt^2-a^2(t)(d\chi^2+r^2d\phi^2).} @node Extending distance concepts to 3D, Invoking astcosmiccal, Distance on a 2D curved space, CosmicCalculator @subsection Extending distance concepts to 3D The concepts of @ref{Distance on a 2D curved space} are here extended to a 3D space that @emph{might} be curved in a 4D space. We can start with the generic infinitesimal distance in a static 3D universe, but this time not in spherical coordinates instead of polar coordinates. @mymath{\theta} is shown in @ref{sphericalplane}, but here we are 3D beings, positioned on @mymath{O} (the center of the sphere) and the point @mymath{O} is tangent to a 4D-sphere. In our 3D space, a generic infinitesimal displacement will have the distance: @dispmath{ds_s^2=dx^2+dy^2+dz^2=dr^2+r^2(d\theta^2+\sin^2{\theta}d\phi^2).}Like our 2D friend before, we now have to assume an abstract dimension which we cannot visualize. Let's call the fourth dimension @mymath{w}, then the general change in coordinates in the @emph{full} four dimensional space will be: @dispmath{ds_s^2=dr^2+r^2(d\theta^2+\sin^2{\theta}d\phi^2)+dw^2.}But we can only work on a 3D curved space, so following exactly the same steps and conventions as our 2D friend, we arrive at: @dispmath{ds_s^2={dr^2\over 1-Kr^2}+r^2(d\theta^2+\sin^2{\theta}d\phi^2).}In a non-static universe (with a scale factor a(t), the distance can be written as: @dispmath{ds^2=c^2dt^2-a^2(t)[d\chi^2+r^2(d\theta^2+\sin^2{\theta}d\phi^2)].} @c@dispmath{H(z){\equiv}\left(\dot{a}\over a\right)(z)=H_0E(z) } @c@dispmath{E(z)=[ \Omega_{\Lambda,0} + \Omega_{C,0}(1+z)^2 + @c\Omega_{m,0}(1+z)^3 + \Omega_{r,0}(1+z)^4 ]^{1/2}} @c Let's take @mymath{r} to be the radial coordinate of the emitting @c source, which emitted its light at redshift $z$. Then the comoving @c distance of this object would be: @c@dispmath{ \chi(r)={c\over H_0a_0}\int_0^z{dz'\over E(z')} } @c@noindent @c So the proper distance at the current time to that object is: @c @mymath{a_0\chi(r)}, therefore the angular diameter distance @c (@mymath{d_A}) and luminosity distance (@mymath{d_L}) can be written @c as: @c@dispmath{ d_A={a_0\chi(r)\over 1+z}, \quad d_L=a_0\chi(r)(1+z) } @node Invoking astcosmiccal, , Extending distance concepts to 3D, CosmicCalculator @subsection Invoking CosmicCalculator CosmicCalculator will calculate cosmological variables based on the input parameters. The executable name is @file{astcosmiccal} with the following general template @example $ astcosmiccal [OPTION...] ... @end example @noindent One line examples: @example $ astcosmiccal --onlyvolume -z 0.8 $ astcosmiccal -l0.6964 -m0.3036 -z2.1 $ astcosmiccal --olambda=0.6964 --omatter=0.3036 --redshift=2.1 @end example The input parameters can be given as command-line options or in the configuration files, see @ref{Configuration files}. For a definition of the different parameters, please see the sections prior to this. By default, all the cosmological calculations will be printed in the standard output (the command-line mainly) along with a short description and units. The options starting with @option{--only} will only do that single desired calculation and only print the final number (in the same units as reported by default). These options are very useful when you want to call CosmicCalculator from a script. The resulting number can simply be put into a shell variable (for example @code{vol}) with the following line, which will allow you to use the value for any other subsequent operation. @example z=3.12 vol=$(astcosmiccal --redshift=$z --onlyvolume) @end example @cindex GNU Grep @noindent In a script, this operation might be necessary for a very large number of objects (thousands of galaxies in a catalog for example). So the fact that all the other default calculations are ignored will also help you get to your result faster. If you just want to inspect the value of a variable, the description (which comes with units) might be more useful. In that case, the following command might be better. The other parameters will also be calculated, but they are so fast that you will not notice on modern computers. @example $ astcosmiccal --redshift=0.832 | grep volume @end example @noindent The full list of options is shown and described below: @table @option @item -z @itemx --redshift (@option{=FLT}) The redshift of interest. @item -H @itemx --H0 (@option{=FLT}) Current expansion rate (in km sec@mymath{^{-1}} Mpc@mymath{^{-1}}). @item -l @itemx --olambda (@option{=FLT}) Cosmological constant density divided by the critical density in the current Universe (@mymath{\Omega_{\Lambda,0}}). @item -m @itemx --omatter (@option{=FLT}) Matter (including massive neutrinos) density divided by the critical density in the current Universe (@mymath{\Omega_{m,0}}). @item -r @itemx --oradiation (@option{=FLT}) Radiation density divided by the critical density in the current Universe (@mymath{\Omega_{r,0}}). @item -v @itemx --onlyvolume Only print the comoving volume (in units of Mpc@mymath{^3}) until the desired redshift based on the input parameters. See explanations above for more on these types of options and how to effectively use them. @item -d @itemx --onlyabsmagconv Only print the conversion factor for apparent magnitude to absolute magnitude. Note that this is practically the distance modulus added with @mymath{-2.5\log{(1+z)}} for the the desired redshift based on the input parameters. See explanations above for more on these types of options and how to effectively use them. @end table @node Libraries, Developing, High-level calculations, Top @chapter Libraries Each program in Gnuastro that was discussed in the prior chapters (or any program in general) is a collection of functions that is compiled into one executable file which can communicate directly with the outside world. The outside world in this context is the operating system. By communication, we mean that control is directly passed to a program from the operating system with a (possible) set of inputs and after it is finished, the program will pass control back to the operating system. For programs written in C and C++, the unique @code{main} function is in charge of this communication. Similar to a program, a library is also a collection of functions that is compiled into one executable file. However, unlike programs, libraries don't have a @code{main} function. Therefore they can't communicate directly with the outside world. This gives you the chance to write your own @code{main} function and call library functions from within it. After compiling your program into a binary executable, you just have to @emph{link} it to the library and you are ready to run (execute) your program. In this way, you can use Gnuastro at a much lower-level, and in combination with other libraries on your system, you can significantly boost your creativity. This chapter starts with a basic introduction to libraries and how you can use them in @ref{Review of library fundamentals}. The separate functions in the Gnuastro library are then introduced (classified by context) in @ref{Gnuastro library}. If you end up routinely using a fixed set of library functions, with a well-defined input and output, it will be much more beneficial if you define a program for the job. Therefore, in its @ref{Version controlled source}, Gnuastro comes with the @ref{The TEMPLATE program} to easily define your own programs(s). @menu * Review of library fundamentals:: Guide on libraries and linking. * Gnuastro library:: Description of all library functions. @end menu @node Review of library fundamentals, Gnuastro library, Libraries, Libraries @section Review of library fundamentals Gnuastro's libraries are written in the C programming language. In @ref{Why C}, we have thoroughly discussed the reasons behind this choice. C was actually created to write Unix, thus understanding the way C works can greatly help in effectively using programs and libraries in all Unix-like operating systems. Therefore, in the following subsections some important aspects of C, as it relates to libraries (and thus programs that depend on them) on Unix are reviewed. First we will discuss header files in @ref{Headers} and then go onto @ref{Linking}. This section finishes with @ref{Summary and example on libraries}. If you are already familiar with these concepts, please skip this section and go directly to @ref{Gnuastro library}. @cindex Modularity In theory, a full operating system (or any software) can be written as one function. Such a software would not need any headers or linking (that are discussed in the subsections below). However, writing that single function and maintaining it (adding new features, fixing bugs, documentation and etc) would be a programmer or scientist's worst nightmare! Furthermore, all the hard work that went into creating it cannot be reused in other software: every other programmer or scientist would have to re-invent the wheel. The ultimate purpose behind libraries (which come with headers and have to be linked) is to address this problem and increase modularity: ``the degree to which a system's components may be separated and recombined'' (from Wikipedia). The more modular the source code of a program or library, the easier maintaining it will be, and all the hard work that went into creating it can be reused for a wider range of problems. @menu * Headers:: Header files included in source. * Linking:: Linking the compiled source files into one. * Summary and example on libraries:: A summary and example on using libraries. * Automatic linking script:: Shell function for automatic linking. @end menu @node Headers, Linking, Review of library fundamentals, Review of library fundamentals @subsection Headers @cindex Pre-Processor C source code is read from top to bottom in the source file, therefore program components (for example variables, data structures and functions) should all be @emph{defined} or @emph{declared} closer to the top of the source file: before they are used. @emph{Defining} something in C or C++ is jargon for providing its full details. @emph{Declaring} it, on the other-hand, is jargon for only providing the minimum information needed for the compiler to pass it temporarily and fill in the detailed definition later. For a function, the @emph{declaration} only contains the inputs and their data-types along with the output's type@footnote{Recall that in C, functions only have one output.}. The @emph{definition} adds to the declaration by including the exact details of what operations are done to the inputs to generate the output. As an example, take this simple summation function: @example double sum(double a, double b) @{ return a + b; @} @end example @noindent What you see above is the @emph{definition} of this function: it shows you (and the compiler) exactly what it does to the two @code{double} type inputs and that the output also has a @code{double} type. Note that a function's internal operations are rarely so simple and short, it can be arbitrarily long and complicated. This unreasonably short and simple function was chosen here for ease of reading. The declaration for this function is: @example double sum(double a, double b); @end example @noindent You can think of a function's declaration as a building's address in the city, and the definition as the building's complete blueprints. When the compiler confronts a call to a function during its processing, it doesn't need to know anything about how the inputs are processed to generate the output. Just as the postman doesn't need to know the inner structure of a building when delivering the mail. The declaration (address) is enough. Therefore by @emph{declaring} the functions once at the start of the source files, we don't have to worry about @emph{defining} them after they are used. Even for a simple real-world operation (not a simple summation like above!), you will soon need many functions (for example, some for reading/preparing the inputs, some for the processing, and some for preparing the output). Although it is technically possible, managing all the necessary functions in one file is not easy and is contrary to the modularity principle (see @ref{Review of library fundamentals}), for example the functions for preparing the input can be usable in your other projects with a different processing. Therefore, as we will see later (in @ref{Linking}), the functions don't necessarily need to be defined in the source file where they are used. As long as their definitions are ultimately linked to the final executable, everything will be fine. For now, it is just important to remember that the functions that are called within one source file must be declared within the source file (declarations are mandatory), but not necessarily defined there. In the spirit of modularity, it is common to define contextually similar functions in one source file. For example, in Gnuastro, functions that calculate the median, mean and other statistical functions are defined in @file{lib/statistics.c}, while functions that deal directly with FITS files are defined in @file{lib/fits.c}. Keeping the definition of similar functions in a separate file greatly helps their management and modularity, but this fact alone doesn't make things much easier for the caller's source code: recall that while definitions are optional, declarations are mandatory. So if this was all, the caller would have to manually copy and paste (@emph{include}) all the declarations from the various source files into the file they are working on now. To address this problem, programmers have adopted the header file convention: the header file of a source code contains all the declarations that a caller would need to be able to use any of its functions. For example, in Gnuastro, @file{lib/statistics.c} (file containing function definitions) comes with @file{lib/gnuastro/statistics.h} (only containing function declarations). The discussion above was mainly focused on functions, however, there are many more programming constructs such as pre-processor macros and data structures. Like functions, they also need to be known to the compiler when it confronts a call to them. So the header file also contains their definitions or declarations when they are necessary for the functions. @cindex Macro @cindex Structures @cindex Data structures @cindex Pre-processor macros Pre-processor macros (or macros for short) are replaced with their defined value by the pre-processor before compilation. Conventionally they are written only in capital letters to be easily recognized. It is just important to understand that the compiler doesn't see the macros, it sees their fixed values. So when a header specifies macros you can do your programming without worrying about the actual values. The standard C types (for example @code{int}, or @code{float}) are very low-level and basic. We can collect multiple C types into a @emph{structure} for a higher-level way to keep and pass-along data. See @ref{FITS macros and data structures} for some examples of macros and data structures. The contents in the header need to be @emph{include}d into the caller's source code with a special pre-processor command: @code{#include }. As the name suggests, the @emph{pre-processor} goes through the source code prior to the processor (or compiler). One of its jobs is to include, or merge, the contents of files that are mentioned with this directive in the source code. Therefore the compiler sees a single entity containing the contents of the main file and all the included files. This allows you to include many (sometimes thousands of) declarations into your code with only one line. Since the headers are also installed with the library into your system, you don't even need to keep a copy of them for each separate program, making things even more convenient. Try opening some of the @file{.c} files in Gnuastro's @file{lib/} directory with a text editor to check out the include directives at the start of the file (after the copyright notice). Let's take @file{lib/fits.c} as an example. You will notice that Gnuastro's header files (like @file{gnuastro/fits.h}) are indeed within this directory (the @file{fits.h} file is in the @file{gnuastro/} directory). You will notice that files like @file{stdio.h}, or @file{string.h} are not in this directory (or anywhere within Gnuastro). On most systems the basic C header files (like @file{stdio.h} and @file{string.h} mentioned above) are located in @file{/usr/include/}@footnote{The @file{include/} directory name is taken from the pre-processor's @code{#include} directive, which is also the motivation behind the `I' in the @option{-I} option to the pre-processor.}. Your compiler is configured to automatically search that directory (and possibly others), so you don't have to explicitly mention these directories. Go ahead, look into the @file{/usr/include} directory and find @file{stdio.h} for example. When the necessary header files are not in those specific libraries, the pre-processor can also search in places other than the current directory. You can specify those directories with this pre-processor option@footnote{Try running Gnuastro's @command{make} and find the directories given to the compiler with the @option{-I} option.}: @table @option @item -I DIR ``Add the directory @file{DIR} to the list of directories to be searched for header files. Directories named by '-I' are searched before the standard system include directories. If the directory @file{DIR} is a standard system include directory, the option is ignored to ensure that the default search order for system directories and the special treatment of system headers are not defeated...'' (quoted from the GNU Compiler Collection manual). Note that the space between @key{I} and the directory is optional and commonly not used. @end table If the pre-processor can't find the included files, it will abort with an error. In fact a common error when building programs that depend on a library is that the compiler doesn't not know where a library's header is (see @ref{Known issues}). So you have to manually tell the compiler where to look for the library's headers with the @option{-I} option. For a small software with one or two source files, this can be done manually (see @ref{Summary and example on libraries}). However, to enhance modularity, Gnuastro (and most other bin/libraries) contain many source files, so the compiler is invoked many times@footnote{Nearly every command you see being executed after running @command{make} is one call to the compiler.}. This makes manual addition or modification of this option practically impossible. @cindex GNU build system @cindex @command{CPPFLAGS} To solve this problem, in the GNU build system, there are conventional environment variables for the various kinds of compiler options (or flags). These environment variables are used in every call to the compiler (they can be empty). The environment variable used for the C Pre-Processor (or CPP) is @command{CPPFLAGS}. By giving @command{CPPFLAGS} a value once, you can be sure that each call to the compiler will be affected. See @ref{Known issues} for an example of how to set this variable at configure time. @cindex GNU build system As described in @ref{Installation directory}, you can select the top installation directory of a software using the GNU build system, when you @command{./configure} it. All the separate components will be put in their separate sub-directory under that, for example the programs, compiled libraries and library headers will go into @file{$prefix/bin} (replace @file{$prefix} with a directory), @file{$prefix/lib}, and @file{$prefix/include} respectively. For enhanced modularity, libraries that contain diverse collections of functions (like GSL, WCSLIB, and Gnuastro), put their header files in a sub-directory unique to themselves. For example all Gnuastro's header files are installed in @file{$prefix/include/gnuastro}. In your source code, you need to keep the library's sub-directory when including the headers from such libraries, for example @code{#include }@footnote{the top @file{$prefix/include} directory is usually known to the compiler}. Not all libraries need to follow this convention, for example CFITSIO only has one header (@file{fitsio.h}) which is directly installed in @file{$prefix/include}. @node Linking, Summary and example on libraries, Headers, Review of library fundamentals @subsection Linking @cindex GNU Libtool To enhance modularity, similar functions are defined in one source file (with a @file{.c} suffix, see @ref{Headers} for more). After running @command{make}, each human-readable, @file{.c} file is translated (or compiled) into a computer-readable ``object'' file (ending with @file{.o}). Note that object files are also created when building programs, they aren't particular to libraries. Try opening Gnuastro's @file{lib/} and @file{bin/progname/} directories after running @command{make} to see these object files@footnote{Gnuastro uses GNU Libtool for portable library creation. Libtool will also make a @file{.lo} file for each @file{.c} file when building libraries (@file{.lo} files are human-readable).}. Afterwards, the object files are @emph{linked} together to create an executable program or a library. @cindex GNU Binutils The object files contain the full definition of the functions in the respective @file{.c} file along with a list of any other function (or generally ``symbol'') that is referenced there. To get a list of those functions you can use the @command{nm} program which is part of GNU Binutils. For example from the top Gnuastro directory, run: @example $ nm bin/arithmetic/arithmetic.o @end example @noindent This will print a list of all the functions (more generally, `symbols') that were called within @file{bin/arithmetic/arithmetic.c} along with some further information (for example a @code{T} in the second column shows that this function is actually defined here, @code{U} says that it is undefined here). Try opening the @file{.c} file to check some of these functions for your self. Run @command{info nm} for more information. @cindex Static linking @cindex Linking: Static To recap, the @emph{compiler} created the separate object files mentioned above for each @file{.c} file. The @emph{linker} will then combine all the symbols of the various object files (and libraries) into one program or library. In the case of Arithmetic (a program) the contents of the object files in @file{bin/arithmetic/} are copied (and re-ordered) into one final executable file which we can run from the operating system. When the symbols (computer-readable function definitions in most cases) are copied into the output like this, we call the process @emph{static} linking. Let's have a closer look at static linking: we'll assume you have installed Gnuastro into the default @file{/usr/local/} directory (see @ref{Installation directory}). If you tried the @command{nm} command on one of Arithmetic's object files above, then with the command below you can confirm that all the functions that were defined in the object files (had a @code{T} in the second column) are also defined in the @file{astarithmetic} executable: @example $ nm /usr/local/bin/astarithmetic @end example @noindent But you will notice that there are still many undefined symbols (have a @code{U} in the second column). One class of such functions are Gnuastro's own library functions that start with `@code{gal_}': @example $ nm /usr/local/bin/astarithmetic | grep gal_ @end example @cindex GNU Libtool @cindex Shared library @cindex Library: shared @cindex Dynamic linking @cindex Linking: dynamic These undefined symbols (functions) will be linked to the executable every time you run arithmetic. Therefore they are known as dynamically @emph{linked} libraries @footnote{Do not confuse dynamically @emph{linked} libraries with dynamically @emph{loaded} libraries. The former (that is discussed here) are only loaded once at the program startup. However, the latter can be loaded anytime during the program's execution, they are also known as plugins.}. When the functions of a library need to be dynamically linked, the library is known as a shared library. As we saw above, static linking is done when the executable is being built. However, when a library is linked dynamically, its symbols are only checked with the available libraries at build time: they are not actually copied into the executable. Every time you run the program, the linker will be activated and will try to link the program to the installed library before it starts. If you want all the libraries to be statically linked to the executables, you have to tell Libtool (which Gnuastro uses for the linking) to disable shared libraries at configure time@footnote{Libtool is very common and is commonly used. Therefore, you can use this option to configure on most programs using the GNU build system if you want static linking.}: @example $ configure --disable-shared @end example @noindent Try configuring, statically building and installing Gnuastro with the command above. Then check the @code{gal_} symbols in the installed Arithmetic executable like before. You will see that they are actually copied this time (have a @code{T} in the second column). If the second column doesn't convince you, look at the executable file size with the following command: @example $ ls -lh /usr/local/bin/astarithmetic @end example @noindent It should be around 4.2 Megabytes with this static linking. If you configure and build Gnuastro again with shared libraries enabled (which is the default), you will notice that it is roughly 100 Kilobytes! This huge difference would have been very significant in the old days, but with the roughly Terabyte storages commonly in use today, it is negligible. Fortunately, output file size is not the only benefit of dynamic linking: since it links to the libraries at run-time (rather than build-time), you don't have to re-build a higher-level program or library when an update comes for one of the lower-level libraries it depends on. You just install the new low-level library and it will automatically be used next time in your higher-level tools. To be fair, this also creates a few complications@footnote{Both of these can be avoided by joining the mailing lists of the lower-level libraries and checking the changes in newer versions before installing them. Updates that result in such behaviors are generally heavily emphasized in the release notes.}: @itemize @item Reproducibility: Even though your high-level tool has the same version as before, with the updated library, you might not get the same results. @item Broken links: if some functions have been changed or removed in the updated library, then the linker will abort with an error at run-time. Therefore you need to re-build your higher-level program or library. @end itemize @cindex GNU C library To see a list of all the shared libraries that are needed for a program or a shared library to run, you can use the GNU C library's @command{ldd}@footnote{If your operating system is not using the GNU C library, you might need another tool.} program, for example: @example $ ldd /usr/local/bin/astarithmetic @end example Library file names start with a @file{lib} and end with suffix depending on their type as described below. In between these two is the name of the library, for example @file{libgnuastro.a} (Gnuastro's static library) and @file{libgsl.so.0.0.0} (GSL's shared library). @itemize @item A static library is known as an archive file and has a @file{.a} suffix. A static library is not an executable file. @item @cindex Shared library versioning @cindex Versioning: Shared library A shared library ends with a @file{.so.X.Y.Z} suffix and is executable. The three numbers in the prefix are the version of the shared library. Shared library versions are defined to allow multiple versions of a shared library simultaneously on a system and to help detect possible updates in the library and programs that depend on it by the linker. It is very important to mention that this version number is different from from the software version number (see @ref{Version numbering}), so do not confuse the two. See the ``Library interface versions'' chapter of GNU Libtool for more. For each shared library, we also have two symbolic links ending with @file{.so.X} and @file{.so}. They are automatically set by the installer, but you can change them (point them to another version of the library) when you have multiple versions on your system. @end itemize @cindex GNU Libtool For those libraries that use GNU Libtool (including Gnuastro and its dependencies), both static and dynamic libraries are built and installed in the @file{prefix/lib/} directory (see @ref{Installation directory}). In this way other programs can make which ever kind of link that they want. To link with a library, the linker needs to know where to find the library. You do that with two separate options to the linker (see @ref{Summary and example on libraries} for an example): @table @option @item -L DIR Will tell the linker to look into @file{DIR} for the libraries. For example @file{-L/usr/local/lib}, or @file{-L/home/yourname/.local/lib}. You can make multiple calls to this option, so the linker looks into several directories. Note that the space between @key{L} and the directory is optional and commonly not used. @item -lLIBRARY Specify the unique name of a library to be linked. As discussed above, library file names have fixed parts which must not be given to this option. So @option{-lgsl} will guide the linker to either look for @file{libgsl.a} or @file{libgsl.so} (depending on the type of linking it is suppose to do). You can link many libraries by repeated calls to this option. @strong{Very important: } The place of this option on the command line matters. This is often a source of confusion for beginners, so let's assume you have asked the linker to link with library A using this option. As soon as the linker confronts this option, it looks into the list of the undefined symbols it has found until that point and does a search in library A for any of those symbols. If any pending undefined symbol is found in library A, it is used. After the search in undefined symbols is complete, the contents of library A are completely discarded from the linker's memory. Therefore, if a later object file or library uses an unlinked symbol in library A, the linker will abort after it has finished its search in all the input libraries or object files. As an example, Gnuastro's @code{gal_array_dlog10_array} function depends on the @code{log10} function of the C Math library (specified with @option{-lm}). So the proper way to link something that uses this function is @option{-lgnuastro -lm}. If instead, you give: @option{-lm -lgnuastro} the linker will complain and abort. @end table @node Summary and example on libraries, Automatic linking script, Linking, Review of library fundamentals @subsection Summary and example on libraries After the mostly abstract discussions of @ref{Headers} and @ref{Linking}, we'll give a small tutorial here. But before that, let's recall the general steps of how your source code is prepared, compiled and linked to the libraries it depends on so you can run it: @enumerate @item The @strong{pre-processor} includes the header (@file{.h}) files into the function definition (@file{.c}) files, expands pre-processor macros and generally prepares the human-readable source for compilation (reviewed in @ref{Headers}). @item The @strong{compiler} will translate (compile) the human-readable contents of each source (merged @file{.c} and the @file{.h} files, or generally the output of the pre-processor) into the computer-readable code of @file{.o} files. @item The @strong{linker} will link the called function definitions from various compiled files to create one unified object. When the unified product has a @code{main} function, this function is the product's only entry point, enabling the operating system or user to directly interact with it, so the product is a program. When the product doesn't have a @code{main} function, the linker's product is a library and its exported functions can be linked to other executables (it has many entry points). @end enumerate @cindex GCC @cindex GNU Compiler Collection The GNU Compiler Collection (or GCC for short) will do all three steps. So as a first example, from Gnuastro's source, go to @file{tests/lib/}. This directory contains the library tests, you can use these as some simple tutorials. For this demonstration, we will compile and run the @file{arraymanip.c}. This small program will call Gnuastro library for some simple operations on an array (open it and have a look). To compile this program, run this command inside the directory containing it. @example $ gcc arraymanip.c -lgnuastro -lm -o arraymanip @end example @noindent The two @option{-lgnuastro} and @option{-lm} options (in this order) tell GCC to first link with the Gnuastro library and then with C's math library. The @option{-o} option is used to specify the name of the output executable, without it the output file name will be @file{a.out} (on most OSs), independent of your input file name(s). If your top Gnuastro installation directory (let's call it @file{$prefix}, see @ref{Installation directory}) is not recognized by GCC, you will get pre-processor errors for unknown header files. Once you fix it, you will get linker errors for undefined functions. To fix both, you should run GCC as follows: additionally telling it which directories it can find Gnuastro's headers and compiled library (see @ref{Headers} and @ref{Linking}): @example $ gcc -I$prefix/include -L$prefix/lib arraymanip.c -lgnuastro -lm \ -o arraymanip @end example @noindent This single command has done all the pre-processor, compilation and linker operations. Therefore no intermediate files (object files in particular) were created, only a single output executable was created. You are now ready to run the program with: @example $ ./arraymanip @end example The Gnuastro functions called by this program only needed to be linked with the C math library. But if your program needs WCS coordinate transformations, needs to read a FITS file, needs special math operations (which include its linear algebra operations), or you want it to run on multiple CPU threads, you also need to add these libraries in the call to GCC: @option{-lgnuastro -lwcs -lcfitsio -lgsl -lgslcblas -pthread -lm}. In @ref{Gnuastro library}, where each function is documented, it is mentioned which libraries (if any) must also be linked when you call a function. If you feel all these linkings can be confusing, please have a look at @ref{Automatic linking script}. @node Automatic linking script, , Summary and example on libraries, Review of library fundamentals @subsection Automatic linking script The number and order of libraries that are necessary for linking a program with Gnuastro library might be too confusing when you need to compile a small program for one particular job (with one source file). To solve this problem, please add these lines to your @file{~/.bashrc} with a text editor and replace @code{PREFIX} with Gnuastro's installation directory (see @ref{Installation directory}). @example # Compile and correctly link Gnuastro related programs function gnuastro-gcc @{ libtool --mode=link gcc $1.c $2 PREFIX/lib/libgnuastro.la -o $1 @} @end example @cindex GNU Libtool This tiny shell function uses GNU Libtool to find the necessary libraries to link against. Libtool uses the same libraries that were checked when you configured Gnuastro to link your program. So in the future, if Gnuastro's prerequisite libraries change, you don't have to worry. Afterwards, when you want to compile a C program that uses Gnuastro library (for example @file{myprog.c}), just run the following command from the directory which contains the source file: @example gnuastro-gcc myprog @end example @noindent If your program needs to link with libraries other than those needed by Gnuastro, you can specify them as a second argument (within double quotes): @example gnuastro-gcc myprog "-lfirst -lsecond" @end example @noindent If you also want to execute the compiled program without typing a second command, add @command{&& ./myprog} to either of the lines above, like the example below. If your program can take arguments, then you can also include them afterwards. @example gnuastro-gcc myprog && ./myprog @end example @node Gnuastro library, , Review of library fundamentals, Libraries @section Gnuastro library Gnuastro library's exported constructs (functions, macros, data structures, or global variables) are classified by context into multiple header files (see @ref{Headers})@footnote{Within Gnuastro's source, all installed @file{.h} files in @file{lib/gnuastro/} are accompanied by a @file{.c} file in @file{/lib/}.}. In this section, the functions in each header will be discussed under a separate sub-section, which includes the name of the header. Assuming a function declaration is in @file{headername.h}, you can include its declaration in your source code with: @example # include @end example @noindent The names of all constructs are prefixed with @code{gal_headername_} (or @code{GAL_HEADERNAME_} for macros). The @code{gal_} prefix stands for @emph{G}NU @emph{A}stronomy @emph{L}ibrary. The @code{headername} prefix is replaced by the header file name (without the @file{.h}) which contains the construct. All Gnuastro library functions are compiled into a single file which can be linked on the command-line with the @option{-lgnuastro} option, (see @ref{Linking} and @ref{Summary and example on libraries} for an introduction). Gnuastro library is a high-level library which depends on lower level libraries for some operations (see @ref{Dependencies}). Therefore if at least one of Gnuastro's functions in your program use functions from the dependencies, you will also need to link those dependencies after linking with Gnuastro. The outside libraries that need to be linked for such functions are mentioned following the function name. See @ref{Automatic linking script} for a small shell function to worry about the libraries to link against and let you focus on your exciting science. @cartouche @noindent @strong{Libraries are still under heavy development: } Gnuastro was initially created to be a collection of command-line programs. However, as the programs and their the shared functions grew, internal (not installed) libraries were added. With the 0.2 release, the libraries are install able. Because of this history in these early phases, the libraries are not fully programmer friendly yet: they abort the program on an error, their naming and arguments are not fully uniform, or modular, and most of the interesting functions (that are currently only used within one program) are still internal to the program. During the next releases, Gnuastro's library structure will undergo significant evolution to address all these problems. It will stabilize with the removal of this notice. Check the @file{NEWS} file for interface changes. @end cartouche @menu * Installation information:: General information about the installation. * Array manipulation:: Functions for manipulating arrays. * Bounding box:: Finding the bounding box. * FITS files:: Working with FITS data. * Git wrappers:: Wrappers for functions in libgit2. * Linked lists:: Various types of linked lists. * Mesh grid for an image:: Breaking an image into a grid. * Polygons:: Working with the vertices of a polygon. * Qsort functions:: Helper functions for Qsort. * Spatial convolution:: Doing spatial convolution on an image * Statistical operations:: Functions for basic statistics. * Multithreaded programming:: Facilitating use of pthreads. * Text table into a C array:: Read an ASCII text table into a C array. * World Coordinate System:: Dealing with the world coordinate system. @end menu @node Installation information, Array manipulation, Gnuastro library, Gnuastro library @subsection Installation information (@file{gnuastro.h}) The @file{gnuastro/gnuastro.h} header contains information about the full Gnuastro installation on your system. Gnuastro developers should note that this is the only header that is not available within Gnuastro, it is only available to a Gnuastro library user @emph{after} installation. Within Gnuastro, @file{config.h} (which is included in every Gnuastro @file{.c} file, see @ref{Coding conventions}) should have more than enough information about the overall Gnuastro installation. @deffn Macro GAL_GNUASTRO_VERSION This macro can be used as a string literal@footnote{@url{https://en.wikipedia.org/wiki/String_literal}} containing the version of Gnuastro that is being used. See @ref{Version numbering} for the version formats. For example: @example printf("Gnuastro version: %s\n", GAL_GNUASTRO_VERSION); @end example @noindent or @example char *gnuastro_version=GAL_GNUASTRO_VERSION; @end example @end deffn @deffn Macro GAL_GNUASTRO_HAVE_LIBGIT2 Libgit2 is an optional dependency of Gnuastro (see @ref{Optional dependencies}). When it is installed and detected at configure time, this macro will have a value of @code{1}. Otherwise, it will have a value of @code{0}. Gnuastro also comes with some wrappers to make it easier to use libgit2 (see @ref{Git wrappers}). @end deffn @deffn Macro GAL_GNUASTRO_HAVE_PTHREAD_BARRIER The POSIX threads standard define barriers as an optional requirement. Therefore, some operating systems choose to not include it. While installing Gnuastro, we check if your system has this construct and if so, we give this macro a value of @code{1}, otherwise it will have a value of @code{0}. see @ref{Implementation of pthread_barrier} for more. @end deffn @node Array manipulation, Bounding box, Installation information, Gnuastro library @subsection Array manipulation (@file{array.h}) When working on arrays, certain operations are commonly necessary. It is very easy to write a loop for such operations, however such loops can unnecessarily make the code harder to write, read, and debug. So, it is much more cleaner if these operations are defined elsewhere. The declarations of these functions are available in @file{gnuastro/array.h}. In C, an array is a contiguous region of memory. So for most operations here, the dimentionality of the data is irrelevant, we just need the total size of the array. Please note that these functions are still very rudimentary, primarily intended for Gnuastro's internal operations. In future releases, these functions will be updated to be more suitable for a generic library. @deftypefun void gal_array_uchar_init_on_region (unsigned char @code{*in}, const unsigned char @code{v}, size_t @code{start}, size_t @code{s0}, size_t @code{s1}, size_t @code{is1}) Initialize a region of the array @code{in} to the value @code{v}. The region is defined by the 1D index of the first pixel (@code{start}) and its C array (opposite of FITS array) width (@code{s0}) and height (@code{s1}). The full C array width is defined by @code{is1}. @end deftypefun @deftypefun void gal_array_long_init (long @code{*in}, size_t @code{size}, const long @code{v}) Initialize the long type array @code{in} with @code{size} elements to the value @code{v}. @end deftypefun @deftypefun void gal_array_long_init_on_region (long @code{*in}, const long @code{v}, size_t @code{start}, size_t @code{s0}, size_t @code{s1}, size_t @code{is1}) Similar to @code{gal_array_uchar_init_on_region} but for long type arrays. @end deftypefun @deftypefun void gal_array_uchar_copy (unsigned char @code{*in}, size_t @code{size}, unsigned char @code{**out}) Allocate space for and copy the input array @code{in} with @code{size} elements into an output array (@code{out}). @end deftypefun @deftypefun void gal_array_float_copy (float @code{*in}, size_t @code{size}, float @code{**out}) Similar to @code{gal_array_uchar_copy} but for the single precision floating point type. @end deftypefun @deftypefun void gal_array_float_copy_noalloc (float @code{*in}, size_t @code{size}, float @code{*out}) Similar to @code{gal_array_float_copy} but the @code{out} array must already be allocated. @end deftypefun @deftypefun void gal_array_fset_const (float @code{*in}, size_t @code{size}, float @code{a}) Set the input array @code{in} with @code{size} elements to the constant value @code{a}. @end deftypefun @deftypefun void gal_array_freplace_value (float @code{*in}, size_t @code{size}, float @code{from}, float @code{to}) @cindex NaN Replace all elements with value @code{from} to value @code{to} in the @code{in} array with @code{size} elements. @code{from} can be a NaN value, in this case, C's @code{isnan} function is used, not @code{==}. @end deftypefun @deftypefun void gal_array_freplace_nonnans (float @code{*in}, size_t @code{size}, float @code{to}) Replace any non-NaN value in the array @code{in} with @code{size} elements to the value @code{to}. @end deftypefun @deftypefun void gal_array_no_nans (float @code{*in}, size_t @code{*size}) Move all the non-NaN elements in the array @code{in} to the start of the array so that the non-NaN elements are contiguous. This is useful for cases where you want to sort the data. Note that before this function, @code{size} must point to the initial size of the array. After this function returns, size will point to the new size of the array, with only non-Nan elements. @end deftypefun @deftypefun void gal_array_no_nans_double (double @code{*in}, size_t @code{*size}) Similar to @code{gal_array_no_nans} but for double types. @end deftypefun @deftypefun void gal_array_uchar_replace (unsigned char @code{*in}, size_t @code{size}, unsigned char @code{from}, unsigned char @code{to}) Replace all elements with value @code{from} to value @code{to} in the @code{in} array with @code{size} elements. @end deftypefun @deftypefun void gal_array_fmultip_const (float @code{*in}, size_t @code{size}, float @code{a}) Multiply all elements in the float array @code{in} with size @code{size} by the constant @code{a}. @end deftypefun @deftypefun void gal_array_fsum_const (float @code{*in}, size_t @code{size}, float @code{a}) Add all elements in the float array @code{in} with size @code{size} by the constant @code{a}. @end deftypefun @deftypefun {float *} gal_array_fsum_arrays (float @code{*in1}, float @code{*in2}, size_t @code{size}) Add the two arrays @code{in1} and @code{in2} and keep the result in a newly allocated array. The returned value is a pointer to that array. @end deftypefun @deftypefun void gal_array_dmultip_const (double @code{*in}, size_t @code{size}, double @code{a}) Multiply the double type array @code{in} with @code{size} elements with the constant @code{a}. @end deftypefun @deftypefun void gal_array_dmultip_arrays (double @code{*in1}, double @code{*in2}, size_t @code{size}) Multiply the two double type arrays @code{in1} with @code{in2} (both with @code{size} elements) with each other and store the output in the first array. @end deftypefun @deftypefun void gal_array_ddivide_const (double @code{*in}, size_t @code{size}, double @code{a}) Divide the double type array @code{in} with @code{size} elements by the constant @code{a}. @end deftypefun @deftypefun void gal_array_dconst_divide (double @code{*in}, size_t @code{size}, double @code{a}) Divide the constant @code{a} by the array @code{in} with @code{size} and store the result for each pixel in the array. @end deftypefun @deftypefun void gal_array_ddivide_arrays (double @code{*in1}, double @code{*in2}, size_t @code{size}) Divide each element of the two double array @code{in1} by the elements in @code{in2} (both with @code{size} elements) and store the output in the first array. @end deftypefun @deftypefun void gal_array_dsum_const (double @code{*in}, size_t @code{size}, double @code{a}) Add the double type array @code{in} with @code{size} elements with the constant @code{a}. @end deftypefun @deftypefun void gal_array_dsum_arrays (double @code{*in1}, double @code{*in2}, size_t @code{size}) Add the two double type arrays @code{in1} with @code{in2} (both with @code{size} elements) with each other and store the output in the first array. @end deftypefun @deftypefun void gal_array_dsubtract_const (double @code{*in}, size_t @code{size}, double @code{a}) Subtract the double type array @code{in} with @code{size} elements from the constant @code{a}. @end deftypefun @deftypefun void gal_array_dconst_subtract (double @code{*in}, size_t @code{size}, double @code{a}) Subtract the constant @code{a} from the array @code{in} with @code{size} and store the result for each pixel in the array. @end deftypefun @deftypefun void gal_array_dsubtract_arrays (double @code{*in1}, double @code{*in2}, size_t @code{size}) Subtract each element of th the double type array @code{in2} from @code{in1} and put the result in the first array. @end deftypefun @deftypefun void gal_array_dpower_const (double @code{*in}, size_t @code{size}, double @code{a}) Each element in the intput array is taken to the power of of @code{a} and stored in place. @end deftypefun @deftypefun void gal_array_dconst_power (double @code{*in}, size_t @code{size}, double @code{a}) The constant @code{a} is taken to the power of each element in the intput array (@code{in}) and stored in place. @end deftypefun @deftypefun void gal_array_dpower_arrays (double @code{*in1}, double @code{*in2}, size_t @code{size}) Each element in the first input array is taken to the power of the same element in the second array. @end deftypefun @deftypefun void gal_array_dlog_array (double @code{*in1}, size_t @code{size}) The natural logarithm of the input array is taken and stored in place. @end deftypefun @deftypefun void gal_array_dlog10_array (double @code{*in1}, size_t @code{size}) The base-10 logarithm of the input array is taken and stored in place. @end deftypefun @deftypefun void gal_array_dabs_array (double @code{*in1}, size_t @code{size}) Replace each element of the input array with its absolute value. @end deftypefun @node Bounding box, FITS files, Array manipulation, Gnuastro library @subsection Bounding box (@file{box.h}) Functions related to reporting a the bounding box of certain inputs are declared in @file{gnuastro/box.h}. All coordinates in this header are in the FITS format (first axis is the horizontal and the second axis is vertical). @deftypefun void gal_box_ellipse_in_box (double @code{A}, double @code{B}, double @code{theta_rad}, long @code{*width}) Any ellipse can be enclosed into a rectangular box. The purpose of this function is to give the height and width of that box. @code{A} is the ellipse major axis, @code{B} is the minor axis, @code{theta_rad} is the position angle in radians. The @code{width} array will contain the output size in long integer type. @code{width[0]}, and @code{width[1]} are the number of pixels along the first and second FITS axis. @end deftypefun @deftypefun void gal_box_border_from_center (double @code{xc}, double @code{yc}, long @code{*width}, long @code{*fpixel}, long @code{*lpixel}) Given the center (@code{xc} and @code{yc}) and width (two element array) of a box, return the coordinates of the first @code{fpixel} and last @code{lpixel} pixels (both are two element arrays. @end deftypefun @deftypefun int gal_box_overlap (long @code{*naxes}, long @code{*fpixel_i}, long @code{*lpixel_i}, long @code{*fpixel_o}, long @code{*lpixel_o}) We have an image of size @code{naxes} and want to get the overlap of the image with a box. This function will return 1 if there is an overlap and 0 if there isn't. The input and output box are specified by their first and last pixels. When there is an overlap, the coordinates of the first and last pixels of the overlap will be put in @code{fpixel_o} and @code{lpixel_o}. @end deftypefun @node FITS files, Git wrappers, Bounding box, Gnuastro library @subsection FITS files (@file{fits.h}) @cindex FITS @cindex CFITSIO The FITS format is the most common format to store data (images and tables) in astronomy. The CFITSIO library already provides a very good low-level set of functions for manipulating FITS data. Some CFITSIO operations (with well-defined inputs and outputs) are commonly needed in a special order. Therefore Gnuastro comes with the macros, data structures and functions introduced in this section. These functions are actually wrappers around CFITSIO functions for a higher-level (easier) access to FITS data. So if you feel these functions don't exactly do what you want, we strongly recommend reading the CFITSIO manual to use it directly. All the functions and macros introduced in this section are declared in @file{gnuastro/fits.h}. When you include this header, you are also including CFITSIO's @file{fitsio.h} header. So you don't need to explicitly include @file{fitsio.h} anymore and can freely use any of its macros or functions in your code along with those discussed here. In @ref{CFITSIO datatype} we first have a look at the way data types are referenced in CFITSIO (and thus Gnuastro). @ref{FITS macros and data structures} defines the macros and data structures that can be used in functions for a unified format. This subsection finished with @ref{FITS functions}, which introduce the different Gnuastro functions available. @menu * CFITSIO datatype:: Addressing different types of data * FITS macros and data structures:: Gnuastro FITS related macros and structures. * FITS functions:: Functions to work on FITS data. @end menu @node CFITSIO datatype, FITS macros and data structures, FITS files, FITS files @subsubsection CFITSIO @code{datatype} @cindex Data type @cindex Type of data @cindex FITS: data type Data can have multiple types: standards to convert a number of bits (which can only have values of 0 and 1) to different number formats (for example integer or floating point numbers). To store data, the FITS standard defines two major formats: images and tables. An image has a single type for all its data elements (a pixel in a 2D image). A table has a single type for every one of its columns. In both cases, the FITS header stores this information. All the FITS data types correspond to C types (for example @code{short}, @code{int}, @code{float}, or @code{long}). @cindex CFITSIO @cindex @code{BITPIX} In images, the @code{BITPIX} header keyword specifies the type of data in each pixel. Within CFITSIO, the different acceptable values of @code{BITPIX} are stored as macros ending with @code{_IMG}. For example @code{BYTE_IMG}, or @code{DOUBLE_IMG}. See Section 4.1, ``CFITSIO Definitions'', in the CFITSIO manual for the recognized CFITSIO types and their macros. However, the FITS standard also accepts tables: each column in a FITS table has a unique @code{TFORM} header keyword which specifies the type of data in that column. The variety of types in a FITS table can be much larger than an image and thus the standard for identifying them differs. To address these different formats of identifying the type in a uniform infra-structure, CFITSIO identifies a general collection of macros referring to types which can be internally used in all cases (images and tables). Thus in CFITSIO, the variable name @code{datatype} when we are referring to this general collection of types. The image types are a subset of the table column types, so each acceptable @code{datatype} corresponds to one of the table types. The macros for each recognized CFITSIO @code{datatype} start with @code{T}, for example @code{TBYTE}, @code{TDOUBLE}. In CFITSIO (and thus here in Gnuastro), the @code{datatype} is most commonly used, so this variable only accepts one of the accepted @code{T} macros. When the @code{BITPIX} value is desired (as input or output), the variable is called @code{bitpix}. In Gnuastro, the functions @code{gal_fits_bitpix_to_datatype} and @code{gal_fits_tform_to_datatype} are provided to convert @code{bitpix} and @code{tform} values to @code{datatype}. @cartouche @noindent @cindex @file{stdint.h} @strong{CFITSIO integer types:} CFITSIO does not use the standard fixed integer size types of @file{stdint.h}! It uses the subjective @code{short}, @code{int} and @code{long} variables which can differ in size from system to system. For example, the FITS standard defines @code{LONG_IMG} as a 32bit signed integer type, but CFITSIO converts it to a local @code{long} which is 64 bits on a modern (64 bit) machine. To use CFITSIO, we had to adopt the same convention in Gnuastro. This issue can cause confusions, so be careful! @end cartouche @node FITS macros and data structures, FITS functions, CFITSIO datatype, FITS files @subsubsection FITS macros and data structures To facilitate handling of fixed/standard values and store, or pass multiple related variables in your programs, Gnuastro defines the following FITS related macros and data structures, see @ref{Headers} for a more detailed discussion. @deffn Macro GAL_FITS_STRING_BLANK @deffnx Macro GAL_FITS_BYTE_BLANK @deffnx Macro GAL_FITS_LOGICAL_BLANK @deffnx Macro GAL_FITS_SHORT_BLANK @deffnx Macro GAL_FITS_LONG_BLANK @deffnx Macro GAL_FITS_LLONG_BLANK @deffnx Macro GAL_FITS_FLOAT_BLANK @deffnx Macro GAL_FITS_DOUBLE_BLANK @deffnx Macro GAL_FITS_INT_BLANK @deffnx Macro GAL_FITS_SBYTE_BLANK @deffnx Macro GAL_FITS_UINT_BLANK @deffnx Macro GAL_FITS_USHORT_BLANK @deffnx Macro GAL_FITS_ULONG_BLANK @cindex Blank pixel These macros keep Gnuastro's blank value constant for all the recognized datatypes in CFITSIO (see @ref{Blank pixels} for a discussion on blank values). The values for the different types are mostly the lowest or highest possible value for that type (for unsigned types and 8-bit types, the maximum is used). So you can safely ignore the actual value and simply use these values to check. See explanation under the @ref{CFITSIO datatype} function for more on types of data in FITS. @cindex NaN @cindex isnan @cindex IEEE NaN The @code{float} and @code{double} types use the IEEE NaN values and for string it is a @code{NULL} pointer. By definition, a NaN value fails in every condition check, so a NaN value is not equal to itself and the check @code{variable==GAL_FITS_FLOAT_BLANK} will fail even if the value in @code{variable} is NaN. Therefore, to check for blank values in floating point types be careful to use C's @code{isnan} function. @end deffn @deftp Structure gal_fits_key Structure for reading FITS header keywords. This structure will keep the name and value of one keyword. The value will be stored in the element corresponding to the type of the value. When multiple keywords must be read, you can define an array of this structure, for example the following declaration will allocate an array of five keywords to be read. @example struct gal_fits_key keys[5]; @end example The names of the keywords can then be stored separately in the array and this expression will store the values in each element. @example gal_fits_read_keywords("filename.fits", hdu, gal_fits_key, 5); @end example The FITS standard defines a maximum length for the value of keyword, so the space for the @code{str} element is statically allocated (@code{FLEN_VALUE}, which is defined in CFITSIO). So if the string value is necessary where @code{gal_fits_key} is no longer available, then you have to allocate space dynamically and copy the string there. @end deftp @example struct gal_fits_key @{ int status; /* CFITSIO status. */ char *keyname; /* Name of keyword. */ int datatype; /* Type of keyword value. */ char str[FLEN_VALUE]; /* String value. */ unsigned char u; /* Byte value. */ short s; /* Short integer value. */ long l; /* Long integer value. */ LONGLONG L; /* Long Long value. */ float f; /* Float value. */ double d; /* Double value. */ @}; @end example @deftp Structure gal_fits_key_ll @cindex Linked list @cindex last-in-first-out @cindex first-in-first-out Structure for writing FITS keywords. This structure is used for one keyword. However, with the @code{next} element, it can link to another keyword thus creating a linked list to add any number of keywords easily and at any step during your program. Adding new keywords doesn't have to be done manually, the @code{gal_fits_add_to_key_ll} and @code{gal_fits_add_to_key_ll_end} will add new keywords for you to the start or end of the list to make a last-in-first-out or first-in-last-out list. See @ref{Linked lists} for more on the nature of linked lists and more similar structures. @end deftp @example struct gal_fits_key_ll @{ int kfree; /* ==1, free keyword name. */ int vfree; /* ==1, free keyword value. */ int cfree; /* ==1, free comment. */ int datatype; /* Keyword value datatype. */ char *keyname; /* Keyword Name. */ void *value; /* Keyword value. */ char *comment; /* Keyword comment. */ char *unit; /* Keyword unit. */ struct gal_fits_key_ll *next; /* Pointer next keyword. */ @}; @end example @node FITS functions, , FITS macros and data structures, FITS files @subsubsection FITS functions Gnuastro provides the following functions to deal with FITS data related operations. FITS data can have a variety of types, see @ref{CFITSIO datatype} for a discussion on this, in particular the integer variables named @code{datatype}, @code{bitpix}, and @code{tform}. See @ref{FITS macros and data structures} for the structure and macro definitions. @deftypefun void gal_fits_io_error (int @code{status}, char @code{*message}) Report the input or output error as a string and print it along with a short statement that an error in CFITSIO occurred. All CFITSIO functions will change the value of @code{status} if an error occurs. This function will print the CFITSIO error string from the value of @code{status} followed by an optional @code{message} that you can add to it. If the value of @code{message} is @code{NULL}, then a default message will be printed. @end deftypefun @deftypefun int gal_fits_name_is_fits (char @code{*name}) Return @code{1} if the string pointed by @code{name} is a standard FITS filename (or more generally: can be read by CFITSIO) and @code{0} if it isn't. See @ref{Arguments} for the standard FITS filenames. @end deftypefun @deftypefun int gal_fits_suffix_is_fits (char @code{*suffix}) Return @code{1} if the string pointed by @code{suffix} is a standard FITS suffix (or more generally: can be read by CFITSIO) and @code{0} if it isn't. @code{suffix} can contain a dot or not (for example both @file{.fits} and @file{fits} will return @code{1}. See @ref{Arguments} for the standard FITS filenames. @end deftypefun @deftypefun int gal_fits_bitpix_to_datatype (int @code{bitpix}) Return the datatype corresponding to the given @code{bitpix} (value to the @code{BITPIX} header keyword) in a FITS image. @end deftypefun @deftypefun int gal_fits_tform_to_datatype (char @code{tform}) Return the datatype corresponding to the given @code{tform} character of a FITS table column: value to the @code{TFORM} header keyword for the column. Note that in the FITS standard, @code{TFORM} values are characters. @end deftypefun @deftypefun void gal_fits_img_bitpix_size (fitsfile @code{*fptr}, int @code{*bitpix}, long @code{*naxes}) Return the datatype (in FITS @code{BITPIX} format) and image size of a FITS HDU specified with the @code{fitsfile} pointer (defined in CFITSIO). So the HDU must have been already opened. If the number of dimensions is not 2, this function will return an error and abort. @end deftypefun @deftypefun {void *} gal_fits_datatype_blank (int @code{datatype}) Allocate the necessary space and put the blank value of type @code{datatype} in it. Finally, return the pointer to the allocated space. This pointer is commonly necessary when calling CFITSIO read functions as @code{nulval}. See @ref{CFITSIO datatype}. @end deftypefun @deftypefun {void *} gal_fits_datatype_alloc (size_t @code{size}, int @code{datatype}) Allocate an array of @code{size} elements of type @code{datatype}. See @ref{CFITSIO datatype}. @end deftypefun @deftypefun size_t gal_fits_datatype_size (int @code{datatype}) Return the size (in bytes) of the type specified by @code{datatype}, see @ref{CFITSIO datatype}. @end deftypefun @deftypefun void gal_fits_blank_to_value (void @code{*array}, int @code{datatype}, size_t @code{size}, void @code{*value}) Convert the blank values in @code{array} (with @code{size} elements) into the value pointed by @code{value}. @end deftypefun @deftypefun void gal_fits_change_type (void @code{*in}, int @code{inbitpix}, size_t @code{size}, int @code{anyblank}, void @code{**out}, int @code{outbitpix}) Convert the @code{in} array (with @code{inbitpix} type) into an array of type @code{outbitpix} that is pointed by @code{out}. Space will be allocated for the output array within this function. @end deftypefun @deftypefun void gal_fits_num_hdus (char @file{*filename}, int @code{*numhdu}) Find the number of HDUs in @file{filename} and store it in the space pointed to by @code{numhdu}. @end deftypefun @deftypefun void gal_fits_read_hdu (char @code{*filename}, char @code{*hdu}, unsigned char @code{img0_tab1}, fitsfile @code{**outfptr}) Open the HDU @code{hdu} (a string) of the @file{filename} FITS file into the @code{outfptr}. See @option{--hdu} option in @ref{Input output} for the accepted HDU formats. @end deftypefun @deftypefun void gal_fits_read_keywords (char @code{*filename}, char @code{*hdu}, struct gal_fits_key @code{*keys}, size_t @code{num}) Read @code{num} keywords (identified in the @code{keys} array) in the @code{hdu} HDU of @file{filename}. See @ref{FITS macros and data structures} for the definition of @code{gal_fits_key} and its recommended usage with this function. CFITSIO will look for the next keyword starting from the last keyword found. Therefore, it is most efficient to specify the keywords in the same order as they appear in the desired HDU. @end deftypefun @deftypefun void gal_fits_add_to_key_ll (struct gal_fits_key_ll @code{**list}, int @code{datatype}, char @code{*keyname}, int @code{kfree}, void @code{*value}, int @code{vfree}, char @code{*comment}, int @code{cfree}, char @code{*unit}) Add an element to the top of the @code{gal_fits_key_ll} linked list for writing keywords. This structure (or linked list) is used to write FITS keywords and is fully described in @ref{FITS macros and data structures}. Each variable also has the same name as the structure element that is described there. @cindex last-in-first-out Assuming all the keywords were added with this function, you will have a last-in-first-out list: as the the name suggests, the last keyword you add to the list will be the first one that gets popped out and thus written in the FITS file header. @end deftypefun @deftypefun void gal_fits_add_to_key_ll_end (struct gal_fits_key_ll @code{**list}, int @code{datatype}, char @code{*keyname}, int @code{kfree}, void @code{*value}, int @code{vfree}, char @code{*comment}, int @code{cfree}, char @code{*unit}) @cindex first-in-first-out Similar to @code{gal_fits_add_to_key_ll}, except the keyword is added to the end of the list, creating a first-in-first-out list. Therefore the order the keywords are written to the FITS header is the same as the order you have called this function. @end deftypefun @deftypefun void gal_fits_file_name_in_keywords (char @code{*keynamebase}, char @code{*filename}, struct gal_fits_key_ll @code{**list}) Put a filename into the @code{gal_fits_key_ll} list to later write into a HDU header. The FITS standard sets a maximum length for the value of a keyword. This creates problems with file names (including directories), because they can become very long. Therefore, when the filename is longer than the maximum length of a FITS keyword value, this function will break it into several keywords. The @code{keynamebase} string will be appended with a @code{_N} (N>0) and used as the keyword name. @end deftypefun @deftypefun void gal_fits_add_wcs_to_header (fitsfile @code{*fptr}, char @code{*wcsheader}, int @code{nkeyrec}) Add the WCS information into the header of the HDU pointed to by @code{fptr}. The WCS information must already be converted into a long string with the FITS conventions. To help in identifying the WCS information, a few blank lines and a title will be added on top. @end deftypefun @deftypefun void gal_fits_update_keys (fitsfile @code{*fptr}, struct gal_fits_key_ll @code{**keylist}) Given the an opened FITS HDU (pointed to by @code{fptr}), this function will write, or update, all the keywords given in @code{keylist}. See @ref{FITS macros and data structures} for more information on the @code{gal_fits_key_ll} structure or linked list. @end deftypefun @deftypefun void gal_fits_write_keys_version (fitsfile @code{*fptr}, struct gal_fits_key_ll @code{*headers}, char @code{*spack_string}) Write or update (all the) keyword(s) in @code{headers} into the FITS pointer, but also the date, name of your program (@code{spack_string}), along with the versions of Gnuastro, CFITSIO, WCSLIB (when available) into the header, see @ref{Output headers}. Since the data processing depends on the versions of the libraries you have used, it is strongly recommended to include this information in every FITS output. See @ref{FITS macros and data structures} for more information on the @code{gal_fits_key_ll} structure or linked list. @end deftypefun @deftypefun void gal_fits_read_wcs_from_pointer (fitsfile @code{*fptr}, int @code{*nwcs}, struct wcsprm @code{**wcs}, size_t @code{hstartwcs}, size_t @code{hendwcs}) Read the WCSLIB WCS structure (@code{wcs}, and @code{nwcs} the number of WCS structures) from the FITS pointer @code{fptr}. In some cases, it might be necessary to only consider header keywords between a certain range. You can define the range of keywords to look for WCS information with the @code{hstartwcs} and @code{hendwcs} arguments. The range of header keywords will only be considered when the value of @code{hstartwcs} is less than @code{hendwcs}, so if you don't want to limit the range, set both values to 0. After you have finished using the WCS structure, use @code{wcsvfree(&nwcs,&wcs);} to free it. @cartouche @noindent @cindex WCSLIB @cindex Thread-saftey @strong{WCSLIB is not thread-safe: } WCSLIB's @code{wcspih} function is used by to read the FITS keywords into WCSLIB's internal WCS structures. Unfortunately this function is not thread-safe. Therefore, be sure to call that function (or Gnuastro's @code{gal_fits_read_wcs_from_pointer} and @code{gal_fits_read_wcs}) before spinning off threads, see @ref{Multithreaded programming}. @end cartouche @end deftypefun @deftypefun void gal_fits_read_wcs (char @code{*filename}, char @code{*hdu}, size_t @code{hstartwcs}, size_t @code{hendwcs}, int @code{*nwcs}, struct wcsprm @code{**wcs}) Read the WCSLIB WCS structure (@code{wcs} and @code{nwcs} the number of WCS structures) from a FITS file (@code{hdu} in @code{filename}). This is basically just a wrapper around the @code{gal_fits_read_wcs_from_pointer} function, see that function for more. @end deftypefun @deftypefun int gal_fits_hdu_to_array (char @code{*filename}, char @code{*hdu}, int @code{*bitpix}, void @code{**array}, size_t @code{*s0}, size_t @code{*s1}) Read the FITS image (in the @code{hdu} extension of @code{filename}). The image array will be stored in @code{array} and the number of pixels in the first and second C axis will be stored in @code{s0} and @code{s1}. The type of the array will be kept in @code{bitpix}. See @option{--hdu} in @ref{Input output} for the acceptable formats of @code{hdu}. @end deftypefun @deftypefun void gal_fits_array_to_file (char @code{*filename}, char @code{*extname}, int @code{bitpix}, void @code{*array}, size_t @code{s0}, size_t @code{s1}, int @code{anyblank}, struct wcsprm @code{*wcs}, struct gal_fits_key_ll @code{*headers}, char @code{*spack_string}) Write the array @code{array} (with sizes @code{s0} and @code{s1}, type @code{bitpix}, and WCS structure @code{wcs}) into the FITS file @file{filename} and extension name @code{extname}. If the array has any blank pixels, then you can set @code{anyblank} to 1. All the headers in @code{headers} will also be written to this extension and @code{spack_string} is the name of your program (which can include a version number), which will be written in the output header. @end deftypefun @deftypefun void gal_fits_atof_correct_wcs (char @code{*filename}, char @code{*hdu}, int @code{bitpix}, void @code{*array}, size_t @code{s0}, size_t @code{s1}, char @code{*wcsheader}, int @code{wcsnkeyrec}, double @code{*crpix}, char @code{*spack_string}) This is essentially the same as @code{gal_fits_array_to_file}, but through the two element @code{crpix} array, you can change the final @code{CRPIX} keywords that will be written in the FITS file. @end deftypefun @deftypefun void gal_fits_table_size (fitsfile @code{*fitsptr}, size_t @code{*nrows}, size_t @code{*ncols}) Get the number of rows (@code{nrows}) and columns (@code{ncols}) in a FITS table within the @code{fitsptr}. @end deftypefun @deftypefun int gal_fits_table_type (fitsfile @code{*fptr}) Return the type of the table: @code{ASCII_TBL} and @code{BINARY_TBL} for an ASCII or binary table. These two macros are defined by CFITSIO. @end deftypefun @deftypefun void gal_fits_file_or_ext_name (char @code{*inputname}, char @code{*inhdu}, int @code{othernameset}, char @code{**othername}, char @code{*ohdu}, int @code{ohduset}, char @code{*type}) This is mainly a function used in Gnuastro programs. Since a FITS image can have many extensions, usually related data are stored within one FITS file. For example an image, its masked pixels, and the sky standard deviation of the noise are various extensions of one FITS file. It would be very inconvenient if the same file name would have to be repeated in a call to a program for all images that are within one file. To easily manage things, within Gnuastro, each input variable also has an integer variable with the same name, but suffixed with @code{set}. The job of this function is to use the name of the main input image and based on the other arguments, determine what filename should be used for each type. The final argument (@code{type}) is the type of input you want, for example, if you were expecting a mask image, you can give the value @code{"mask"} as type. @code{type} is just used to report errors. @end deftypefun @deftypefun void gal_fits_file_to_float (char @code{*inputname}, char @code{*maskname}, char @code{*inhdu}, char @code{*mhdu}, float @code{**img}, int @code{*inbitpix}, int @code{*anyblank}, size_t @code{*ins0}, size_t @code{*ins1}) Read a FITS image HDU (@code{inhdu} in @file{inputname}) as a @code{float} type array. An optional mask image and mask hdu can also be given. Single precision floating point types are one of the most common types to store data: the observation noise is usually much larger than the extra precision (and thus volume in your computer, and slower processing) offered by double precision floating point types. With this function, so when you work internally with floating points, you can use this function to directly read a FITS image array into a floating point array. @end deftypefun @deftypefun void gal_fits_file_to_double (char @code{*inputname}, char @code{*maskname}, char @code{*inhdu}, char @code{*mhdu}, double @code{**img}, int @code{*inbitpix}, int @code{*anyblank}, size_t @code{*ins0}, size_t @code{*ins1}) Similar to @code{gal_fits_file_to_float}, but for double precision floating point type. In some contexts, the internal operations must be done in double precision floating point types, irrespective of the input type and this function can be used to directly read a file into an array of this type. @end deftypefun @deftypefun void gal_fits_file_to_long (char @code{*inputname}, char @code{*inhdu}, long @code{**img}, int @code{*inbitpix}, int @code{*anyblank}, size_t @code{*ins0}, size_t @code{*ins1}) @cindex Labeled image @cindex Segmentation map Similar to @code{gal_fits_file_to_float}, but will read the image specified by @file{inputname} (@code{inhdu}) into a long integer type. Long integer types are commonly used to store things like segmentation maps or labeled images. @end deftypefun @deftypefun void gal_fits_prep_float_kernel (char @code{*inputname}, char @code{*inhdu}, float @code{**outkernel}, size_t @code{*ins0}, size_t @code{*ins1}) @cindex Convolution kernel @cindex Kernel: convolution Read @file{inputname} (@code{inhdu}) will be read as a floating point array to be used as a convolution kernel. Convolution kernels are commonly necessary in astronomical image processing, but they need to have certain properties: their dimensions have to be an odd number and they must not have any blank pixels. In both cases, this function will abort with an error notice. @end deftypefun @c@deftypefun @c@end deftypefun @node Git wrappers, Linked lists, FITS files, Gnuastro library @subsection Git wrappers (@file{git.h}) @cindex Git @cindex libgit2 Git is one of the most common tools for version control and it can often be useful during development, for example see @code{COMMIT} keyword in @ref{Output headers}. The functions introduced here are described in the @file{gnuastro/git.h} header. At installation time, Gnuastro will also check for the existence of libgit2 and store the value in the @code{GAL_GNUASTRO_HAVE_LIBGIT2}, see @ref{Installation information}. @file{gnuastro/git.h} includes @file{gnuastro/gnuastro.h} internally, so won't have to include both for this macro. @deftypefun {char *} gal_git_describe ( ) When libgit2 is present and the program is called within a directory that is version controlled, then this function will return a string containing the commit description (similar to Gnuastro's unofficial version number, see @ref{Version numbering}). If there are uncommitted changes in the running directory, it will add a `@code{-dirty}' prefix to the description. When there is no tagged point in the previous commit, this function will return a uniquely abbreviated commit object as fallback. This function is used for generating the value of the @code{COMMIT} keyword in @ref{Output headers}. The output string is similar to the output of the following command: @example $ git describe --dirty --always @end example Space for the output string is allocated within this function, so after using the value you have to @code{free} the output string. If libgit2 is not installed or the program calling this function is not within a version controlled directory, then the output will be the @code{NULL} pointer. @end deftypefun @node Linked lists, Mesh grid for an image, Git wrappers, Gnuastro library @subsection Linked lists (@file{linkedlist.h}) @cindex Array @cindex Linked list An array is a contiguous region of memory that is very efficient and easy to use for recording and later accessing the data. One major problem with an array is that the number of elements that go into it must be known in advance. This is where linked lists can be very useful: like a metal chain, each @emph{node} in a linked list is an independent C structure, keeping its own data along with pointer(s) to its immediate neighbor(s). Below we have one simple linked list node structure along with an ASCII art schematic of how we can use the @code{next} pointer to add any number of elements to the list that we want. The linked list is terminated when @code{next} is a @code{NULL} pointer. @c The second and last lines lines are pushed line space forward, because @c the `@{' at the start of the line is only seen as `{' in the book. @example struct float_ll /* --------- --------- */ @{ /* | Value | | Value | */ float value; /* | --- | | --- | */ struct ll_node *next; /* | next-|--> | next-|--> NULL */ @} /* --------- --------- */ @end example The schematic shows another great advantage of linked lists: it is very easy to add or remove a node anywhere in the list (you just have to change one pointer in the structure above). You initially define a variable of this type with a @code{NULL} pointer as shown below, then you use functions provided for that type of linked list to add elements to the list or pop elements from it. @example struct float_ll *mylist=NULL @end example @cindex last-in-first-out @cindex first-in-first-out @noindent When you add an element to the list, it is conventionally added to the ``top'' of the list: the general list pointer will point to the newly created node, which will point to the previously created node and so on. So when you ``pop'' from the top of the list, you are actually retrieving the last value you put in and changing the list pointer to the next oldest node. This is thus known as a ``last-in-first-out'' list. This is the most convenient type of linked list (easier to implement and faster to process). Alternatively, you can add each newly created node at the end of the list. If you do that, you will get a ``first-in-first-out'' list. But that will force you to go through the whole list for each new element that is created (this can slow down the processing)@footnote{A better way to get a first-in-first-out is to first keep the data as last-in-first-out until they are all read. Afterwards, pop each node and immediately add it to the new list: practically reversing the last-in-first-out list to a first-in-first-out one.}. Each node in a linked list doesn't have to have a single pointer to the next node like the example above. We can define each node with two pointers to both the next and previous neighbors, this is called a ``Doubly linked list''. In general, lists are very powerful and simple constructs that can be very useful. But going into more detail would be out of the scope of this short introduction in this book. @url{https://en.wikipedia.org/wiki/Linked_list, Wikipedia} has a nice and more thorough discussion of the various types of lists, so for more, please have a look at that article. In this section we will review the functions and structures that are available in Gnuastro for working on linked lists. For each linked-list node structure, we will first introduce the structure, then the functions for working on the structure. All these structures and functions are defined and declared in @file{gnuastro/linkedlist.h}. @deftp Structure gal_linkedlist_fll Float linked list (@code{fll}). Each node in this singly-linked list can have a single float type value. @end deftp @example struct gal_linkedlist_fll @{ float v; struct gal_linkedlist_fll *next; @}; @end example @deftypefun void gal_linkedlist_print_fll_array (struct gal_linkedlist_fll @code{**afll}, size_t @code{num}) Print all the values within the linked list to the output terminal. This can be used for inspecting the status of the list during development. @end deftypefun @deftypefun void gal_linkedlist_add_to_fll (struct gal_linkedlist_fll @code{**list}, float @code{value}) Allocate space for a new node in @code{list}, and put @code{value} into it. The new node will be added to the top of the list. So after this function, the already existing nodes will be appended to the new node and @code{list} will point to the newly created node. @end deftypefun @deftypefun void gal_linkedlist_pop_from_fll (struct gal_linkedlist_fll @code{**list}, float @code{*value}) Pop a node from the top of @code{list} and put its values in @code{value}. This function will also free the allocated space for the popped node and after this function, @code{list} will point to the next node. @end deftypefun @deftypefun size_t gal_linkedlist_num_in_fll (struct gal_linkedlist_fll @code{*list}) Return the number of nodes in @code{list}, the contents of @code{list} will be untouched. @end deftypefun @deftypefun void gal_linkedlist_fll_to_array (struct gal_linkedlist_fll @code{*list}, float @code{**f}, size_t @code{*num}) Put the elements of @code{list} into an array @code{f} and store the number of nodes in the list in @code{num}. The array will be filled in the same order as popped elements from the list. This function will allocate space for the @code{num} element @code{f} array internally, so you have to free it afterwards. @end deftypefun @deftypefun void gal_linkedlist_free_fll (struct gal_linkedlist_fll @code{*list}) Free the space for all the nodes in @code{list}. Note that any values within the nodes will also be discarded. This can be used when the list is no longer relevant for you. For example, you might have already converted the list to an array for future usage with @code{gal_linkedlist_fll_to_array}. @end deftypefun @deftypefun void gal_linkedlist_free_fll_array (struct gal_linkedlist_fll @code{**afll}, size_t @code{num}) Free an array of @code{gal_linkedlist_fll} linked lists (@code{num} elements). Each element of the array is a pointer to a linked list, so we first need to free the separate linked lists, then the array. @end deftypefun @deftp Structure gal_linkedlist_tdll Two doubles linked list (@code{tdll}. Each node in this singly-linked list can have two double type values. It can be used to store an unknown number of floating point coordinates (for example RA and Dec). @end deftp @example struct gal_linkedlist_tdll @{ double a; double b; struct gal_linkedlist_tdll *next; @}; @end example @deftypefun void gal_linkedlist_add_to_tdll (struct gal_linkedlist_tdll @code{**list}, double @code{a}, double @code{b}) Allocate space for a new node in @code{list}, and put the values @code{a} and @code{b} into it. The new node will be added to the top of the list. So after this function, the already existing nodes will be appended to the new node and @code{list} will point to the newly created node. @end deftypefun @deftypefun void gal_linkedlist_pop_from_tdll (struct gal_linkedlist_tdll @code{**list}, double @code{*a}, double @code{*b}) Pop a node from the top of @code{list} and put its values in @code{a} and @code{b}. This function will also free the allocated space for the popped node and after this function, @code{list} will point to the next node. @end deftypefun @deftypefun size_t gal_linkedlist_num_int_dll (struct gal_linkedlist_tdll @code{*list}) Return the number of nodes in @code{list}. The contents of @code{list} will be untouched. @end deftypefun @deftypefun void gal_linkedlist_tdll_to_array_inv (struct gal_linkedlist_tdll @code{*list}, double @code{**d}, size_t @code{*num}) Put the elements of @code{list} into an array @code{d} in inverse order and store the number of nodes in the list in @code{num}. This function will allocate space for the @mymath{2\times}@code{num} element array internally so you have to free it afterwards. The two values for each node will be stored adjacently, so the array can be seen as a 2D array with @code{num} rows and 2 columns. @end deftypefun @deftypefun void gal_linkedlist_free_tdll (struct gal_linkedlist_tdll @code{*list}) Free the space for all the nodes in @code{list}. Note that any values within the nodes will also be discarded. This can be used when the list is no longer relevant for you. For example, you might have already converted the list to an array for future usage with @code{gal_linkedlist_tdll_to_array_inv}. @end deftypefun @deftp Structure gal_linkedlist_stll String linked list (@code{stll}. Each node in this singly-linked list has a string variable. @end deftp @example struct gal_linkedlist_stll @{ char *v; struct gal_linkedlist_stll *next; @}; @end example @deftypefun void gal_linkedlist_add_to_stll (struct gal_linkedlist_stll @code{**list}, char @code{*value}) Allocate space for a new node in @code{list}, and store the @code{value} pointer into it. The new node will be added to the top of the list. So after this function, the already existing nodes will be appended to the new node and @code{list} will point to the newly created node. It is important to remember that this function will only copy the pointer in the node, it will not allocate space for the string. So the string either has to be a literal string (with a fixed address) or dynamically allocated when this linked list is to be filled and used within one function. @end deftypefun @deftypefun void gal_linkedlist_pop_from_stll (struct gal_linkedlist_stll @code{**list}, char @code{**value}) Pop a node from the top of @code{list} and put its pointer in @code{value}. This function will also free the allocated space for the popped node and after this function, @code{list} will point to the next node. @end deftypefun @deftypefun void gal_linkedlist_reverse_stll (struct gal_linkedlist_stll @code{**list}) Reverse the linked list. The @code{gal_linkedlist_add_to_stll} function will make a last-in-first-out list, but commonly you will need a first-in-first-out list. This function can thus be useful after adding to the list has finished. @end deftypefun @deftypefun void gal_linkedlist_print_stll (struct gal_linkedlist_stll @code{*list}) Print all the values within the linked list to the output terminal. This can be used for inspecting the status of the list during development. @end deftypefun @deftypefun size_t gal_linkedlist_num_in_stll (struct gal_linkedlist_stll @code{*list}) Return the number of nodes in @code{list}. The contents of @code{list} will be untouched. @end deftypefun @deftp Structure gal_linkedlist_sll @cindex @code{size_t} @code{size_t} linked list (@code{sll}. Each node in this singly-linked list contains a @code{size_t} value. The @code{size_t} type is commonly used for ``size'' related values: it is an un-signed type (negative values are not defined for it), therefore it is ideal for dealing with things like pixel indexes in an image (which can not be negative and can be very large). @end deftp @example struct gal_linkedlist_sll @{ size_t v; struct gal_linkedlist_sll *next; @}; @end example @deftypefun void gal_linkedlist_add_to_sll (struct gal_linkedlist_sll @code{**list}, size_t @code{value}) Allocate space for a new node in @code{list}, and store @code{value} into it. The new node will be added to the top of the list. So after this function, the already existing nodes will be appended to the new node and @code{list} will point to the newly created node. @end deftypefun @deftypefun void gal_linkedlist_pop_from_sll (struct gal_linkedlist_sll @code{**list}, size_t @code{*value}) Pop a node from the top of @code{list} and put its value in @code{value}. This function will also free the allocated space for the popped node and after this function, @code{list} will point to the next node. @end deftypefun @deftypefun size_t gal_linkedlist_num_in_sll (struct gal_linkedlist_sll @code{*list}) Return the number of nodes in @code{list}. The contents of @code{list} will be untouched. @end deftypefun @deftypefun void gal_linkedlist_print_sll (struct gal_linkedlist_sll @code{*list}) Print all the values within the linked list to the output terminal. This can be used for inspecting the status of the list during development. @end deftypefun @deftypefun void gal_linkedlist_sll_to_array (struct gal_linkedlist_sll @code{*list}, size_t @code{**s}, size_t @code{*num}, int @code{inverse}) Put the elements of @code{list} into an array @code{s} and store the number of nodes in the list in @code{num}. This function will allocate space for the @code{num} element array internally so you have to free it afterwards. If the value in @code{inverse} is @code{1}, then the first popped value in the list will be the last element in the array, otherwise, the array will be filled in the same order that the elements were popped. @end deftypefun @deftypefun void gal_linkedlist_free_sll (struct gal_linkedlist_sll @code{*list}) Free the space for all the nodes in @code{list}. Note that any values within the nodes will also be discarded. This can be used when the list is no longer relevant for you. For example, you might have already converted the list to an array for future usage with @code{gal_linkedlist_sll_to_array}. @end deftypefun @deftp Structure gal_linkedlist_osll @cindex @code{size_t} Ordered @code{size_t} linked list (@code{osll}. Each node in this singly-linked list contains a @code{size_t} value and a floating point value. The floating point value is used as a reference to add new nodes in a sorted manner. At any moment, the first popped node in this list will have the smallest @code{tosort} value, and subsequent nodes will have larger to values. @end deftp @example struct gal_linkedlist_osll @{ size_t v; float s; struct gal_linkedlist_osll *next; @}; @end example @deftypefun void gal_linkedlist_add_to_osll (struct gal_linkedlist_osll @code{**list}, size_t @code{value}, float @code{tosort}) Allocate space for a new node in @code{list}, and store @code{value} into it. The new node will be added to the list based on the @code{tosort} value. @end deftypefun @deftypefun void gal_linkedlist_pop_from_osll (struct gal_linkedlist_osll @code{**list}, size_t @code{*value}, float @code{*sortvalue}) Pop a node from the top of @code{list}, put its value in @code{value} and its sort value in @code{sortvalue}. This function will also free the allocated space for the popped node and after this function, @code{list} will point to the next node (which has a larger @code{tosort} element). @end deftypefun @deftypefun void gal_linkedlist_osll_into_sll (struct gal_linkedlist_osll @code{*in}, struct gal_linkedlist_sll @code{**out}) Convert the orderd @code{size_t} linked list into an ordinary @code{size_t} linked list (no longer sorted). This can be useful when all the elements have been added and you just need to pop-out elements. @end deftypefun @deftp Structure gal_linkedlist_tosll @cindex @code{size_t} Two-way, ordered @code{size_t} linked list (@code{tosll}. Each node in this Doubly-linked list contains a @code{size_t} value and a floating point value. The floating point value is used as a reference to add new nodes in a sorted manner. In the functions here, this linked list can be pointed to by two pointers (largest and smallest) with the following format: @example largest pointer | NULL <-- (v0,s0) <--> (v1,s1) <--> ... (vn,sn) --> NULL | smallest pointer @end example At any moment, the two pointers will point the nodes containing the ``largest'' and ``smallest'' values and the rest of the nodes will be sorted. This is useful when an unknown number of nodes are being added continuously and during the operations it is important to have the nodes in a sorted format. @end deftp @example struct gal_linkedlist_tosll @{ size_t v; float s; struct gal_linkedlist_tosll *prev; struct gal_linkedlist_tosll *next; @}; @end example @deftypefun void gal_linkedlist_print_tosll (struct gal_linkedlist_tosll @code{*largest}, struct gal_linkedlist_tosll @code{*smallest}) Print all the values within the linked list to the output terminal. This can be used for inspecting the status of the list during development. @end deftypefun @deftypefun void gal_linkedlist_add_to_tosll_end (struct gal_linkedlist_tosll @code{**largest}, struct gal_linkedlist_tosll @code{**smallest}, size_t @code{value}, float @code{tosort}) Allocate space for a new node in @code{list}, and store @code{value} into it. The new node will be added to the list based on the @code{s} value as described in the description of @code{gal_linkedlist_tosll}. If this is the first node to be added to the list, both the @code{largest} and @code{smallest} pointers can be @code{NULL}. @end deftypefun @deftypefun void gal_linkedlist_pop_from_tosll_start (struct gal_linkedlist_tosll @code{**lartest}, struct gal_linkedlist_tosll @code{**smallest}, size_t @code{*value}, float @code{*tosort}) Pop the node with the smallest @code{s} of @code{list}, then put its value in @code{value} and its sort value in @code{sortvalue}. This function will also free the allocated space for the popped node and after this function, @code{largest} and @code{smallest} will be modified respectively. Note that even though only the smallest pointer will be popped, when there was only one node in the list, the @code{largest} pointer also has to change, so we need both. @end deftypefun @deftypefun void gal_linkedlist_smallest_tosll (struct gal_linkedlist_tosll @code{*largest}, struct gal_linkedlist_tosll @code{**smallest}) Given the @code{largest} pointer, set @code{smallest} as described in @code{gal_linkedlist_tosll}. @end deftypefun @deftypefun void gal_linkedlist_tosll_into_sll (struct gal_linkedlist_tosll @code{*in}, struct gal_linkedlist_sll @code{**out}) Convert the two-way orderd @code{size_t} linked list into an ordinary @code{size_t} linked list (no longer sorted). This can be useful when all the elements have been added and you just need to pop-out elements. @end deftypefun @deftypefun void gal_linkedlist_tosll_free (struct gal_linkedlist_tosll @code{*largest}) Free the space for all the nodes in @code{largest}. Note that any values within the nodes will also be discarded. @end deftypefun @node Mesh grid for an image, Polygons, Linked lists, Gnuastro library @subsection Mesh grid for an image (@file{mesh.h}) The basic concepts behind the mesh and channel grids in Gnuastro were explained in @ref{Tiling an image}. Besides the improved measurement purposes introduced there, tiling an image can also greatly speed up some processing operations over the image, since each mesh can be given to a different thread and so the CPU can be working on multiple regions of the image simultaneously. The mesh structure and functions introduced here are declared in @file{gnuastro/mesh.h} and allow you to also use operate on an image mesh. Please note that as discussed in @ref{Gnuastro library}, most library functions will significantly evolve with future releases. The mesh structure and functions introduced here are high on this list: until now they were only internally used and so not much attention had been paid to their usability outside Gnuastro. Gnuastro's @file{lib/mesh.c} contains the full function definitions and is heavily commented, please also consult that file if the explanations here are not clear enough. However, the basic idea behind this structure, and the functions to manipulate data over it, is a powerful tool that can be generically used in many contexts. So please use the structure and functions here very critically and share your criticisms, thoughts and ideas on them. Hopefully in future releases the structure and functions were will evolve to become an easy to use and generically applicable mesh grid system. @deftp Structure gal_mesh_params This structure keeps all the necessary parameters for a particular mesh and channel grid over an image. This structure only keeps the information about the mesh and channel grid structure. It doesn't keep a copy of the different parts of the image. So when working on several images of the same size, you can use the same mesh structure. Its individual elements are too many to fully list here, if you are interested please look into the installed @file{gnuastro/mesh.h} header. One important component of the structure which is commonly used in the functions is the @code{garray}, where each mesh has a unique @code{gid}. @code{garray} stands for grid-array. It is used for operations on the mesh grid, where one value is to be assigned for each mesh. It has one element for each mesh in the image. However, due to the (possible) existence of channels (see @ref{Tiling an image}), each channel needs its own contiguous part (group of meshes) in the full @code{garray}. Each channel has @code{gs0*gs1} (dimensions of meshes in each channel) elements. There are @code{nch} parts (or channels) in total. In short, the meshs in each channel have to be contiguous to facilitate the neighbor analysis in interpolation and other channel specific jobs. So, the over-all structure can be viewed as a 3D array. The operations on the meshs might need more than one output, for example the mean and the standard deviation. So we have two @code{garray}s and two @code{nearest} arrays (for interpolation). @end deftp @deftypefun size_t gal_mesh_ch_based_id_from_gid (struct gal_mesh_params @code{*mp}, size_t @code{gid}) As discussed in the description of @code{gal_mesh_params}, there are two internal ways to refer to a mesh (with an ID): @itemize @item By default, the mesh IDs are set based on their position within the channels (so the meshs in each channel are contiguous). We call this the channel-based mesh ID. The @code{cgarray1} and @code{cgarray2} in @code{gal_mesh_params} store the mesh values based on this ID. All the basic mesh properties, like their types and height and widths are stored based on this ID. @item If the user asks for a full image interpolation or smoothing, then two new arrays are created called @code{fgarray1} and @code{fgarray2}. These arrays keep the mesh values as they appear on the image, irrespective of which channel they belong to. We call this the image-based ID. The image based ID is contiguous over the image. @end itemize The @code{garray1} and @code{garray2} pointers can point to either the @code{cgarrays} or the @code{fgarrays}. Ideally, the user should not worry about what garray is pointing to. The caller knows the type of IDs they are using, but they don't know what to put into @code{garray}. We call the ID that should be put into garray the channel-based ID. It can be either of the two kinds above. So we have the following two functions @code{gal_mesh_ch_based_id_from_gid} and @code{gal_mesh_gid_from_ch_based_id} for changing between these IDs. The former (this function) is used when you are going over the elements in garray (and you are completely ignorant to which one of cgarrays or fgarrays garray points to) and you need the channel based IDs to get basic mesh information like the mesh type and size. @end deftypefun @deftypefun size_t gal_mesh_gid_from_ch_based_id (struct gal_mesh_params @code{*mp}, size_t @code{chbasedid}) See the explanations in @code{gal_mesh_ch_based_id_from_gid} first. This function is used when you are going over the meshs through the channel-based IDs, but you need to know what ID to use for @code{garray}. @end deftypefun @deftypefun size_t gal_mesh_img_xy_to_mesh_id (struct gal_mesh_params @code{*mp}, size_t @code{x}, size_t @code{y}) You have a pixel's position as @code{x} and @code{y} in the final image (in C-based dimensions) and want to know the id to be used in the @code{garray}s to get a value for this pixel in the mesh-grid. This function will return that ID. As an example, you can get the mesh value at a specific position in the image with: @example mp->garray[ gal_mesh_img_xy_to_mesh_id(mp, x, y) ]; @end example @end deftypefun @deftypefun void gal_mesh_check_mesh_id (struct gal_mesh_params @code{*mp}, long @code{**out}) Save the meshid of each pixel into an array the size of the original image. All the pixels over the mesh will get the value of the mesh ID. The output array @code{out} can then be written to a FITS file for viewing. This is mainly used for checking/debugging purposes, hence the @code{check} in the name. @end deftypefun @deftypefun void gal_mesh_check_garray (struct gal_mesh_params @code{*mp}, float @code{**out1}, float @code{**out2}) Save the values in the @code{garray}s of the input @code{mp} structure into two arrays the size of the input image. All the pixels over each mesh will get the value corresponding to that mesh in the @code{garray}s. The output arrays can then be written to a FITS file for viewing. This is mainly used for checking/debugging purposes, hence the @code{check} in the name. @code{out2} will only be set if there are two @code{garray}s. @end deftypefun @deftypefun void gal_mesh_value_file (struct gal_mesh_params @code{*mp}, char @code{*filename}, char @code{*extname1}, char @code{*extname2}, struct wcsprm @code{*wcs}, char @code{*spack_string}) Save the mesh grid values into the @file{filename} FITS file with @code{extname1} and @code{extname2} extension names (for the two possible @code{garrays}), a WCS structure may also optionally be given and @code{spack_string} is the name of your program to be written in the header. The output FITS file will have one pixel for each mesh, so its dimensions will be significantly smaller than the input image. If you want the mesh values in the same dimension as the input image, use @code{gal_mesh_check_garray}. @end deftypefun @deftypefun void gal_mesh_full_garray (struct gal_mesh_params @code{*mp}, int @code{reverse}) As described in @code{gal_mesh_ch_based_id_from_gid}, the there can be two arrays that keep a value for each mesh in @code{gal_mesh_params}: @code{cgarray} and @code{fgarray}. When @code{reverse==0}, then this function will fill in the @code{fgarray}s using the @code{cgarray}s and vice-versa when @code{reverse==1}. @end deftypefun @deftypefun void gal_mesh_make_mesh (struct gal_mesh_params @code{*mp}) Make the mesh structure using the basic information that must already be present within it. The complete list of necessary parameters are as follows, but note that some might not be necessary for your desired functionality. @code{s0}, @code{s1}, @code{ks0}, @code{ks1}, @code{nch1}, @code{nch2}, @code{kernel}, @code{img}, @code{params}, @code{minmodeq}, @code{mirrordist}, @code{fullsmooth}, @code{numnearest}, @code{smoothwidth}, @code{lastmeshfrac}, @code{meshbasedcheck}, @code{interponlyblank}, @code{fullinterpolation}, @code{numthreads}. See the installed @file{gnuastro/mesh.h} for a comment on each parameter within the @code{gal_mesh_params} structure. @end deftypefun @deftypefun void gal_mesh_free_mesh (struct gal_mesh_params @code{*mp}) Free all the allocated spaces within the @code{gal_mesh_params} structure. @end deftypefun @deftypefun void gal_mesh_operate_on_mesh (struct gal_mesh_params @code{*mp}, void @code{*(*meshfunc)(void *)}, size_t @code{oneforallsize}, int @code{makegarray2}, int @code{initialize}) @cindex NaN @cindex Pthread @cindex IEEE NaN Run the @code{meshfunc} function on each mesh in parallel. As the declaration above shows, @code{meshfunc} should only take one @code{void *} input and return one @code{void *} output. This function will setup a pthread environment and make @code{mp->numthreads} (a number!) calls @code{meshfunc} which will work on each mesh. @code{gal_mesh_operate_on_mesh} will return when all the threads have finished their work. If @code{meshfunc} needs to store more than one value for each mesh, then set @code{makegarray2=1}. When @code{initialize==1}, the @code{garray}(s) will be initialized to NaN. This function is commonly used within Gnuastro (mainly in NoiseChisel, see @ref{NoiseChisel}), so search for its applications in the programs for some real-world examples. You can do this with the following command in the top Gnuastro source directory (after unpacking the tarball): @example grep -r gal_mesh_operate_on_mesh ./bin/* @end example @end deftypefun @deftypefun void gal_mesh_interpolate (struct gal_mesh_params @code{*mp}, char @code{*errstart}) @cindex NaN @cindex IEEE NaN Interpolate the mesh values (@code{garray}s). After you have run a function on all the meshes with @code{gal_mesh_operate_on_mesh}, some meshes might not get any values. This function will fill the meshes that didn't get any values (have a value of NaN) using the meshes that received a value. The interpolation is done based on the nearest neighbors, specified within the @code{gal_mesh_params} structure. @end deftypefun @deftypefun void gal_mesh_smooth (struct gal_mesh_params @code{*mp}) Smooth the mesh values arrays based on the parameters in @code{gal_mesh_params}. @end deftypefun @deftypefun void gal_mesh_spatial_convolve_on_mesh (struct gal_mesh_params @code{*mp}, float @code{**conv}) Do spatial convolution (see @ref{Spatial domain convolution}) on each channel of the mesh grid independently, therefore two adjacent pixels within the image that are not in the same channel will not affect each other during the convolution. @end deftypefun @deftypefun void gal_mesh_change_to_full_convolution (struct gal_mesh_params @code{*mp}, float @code{*conv}) After running @code{gal_mesh_spatial_convolve_on_mesh}, it might become necessary to change the convolution into a full image convolution. This function will do the convolution process only on the regions near the channel borders that need to be changed, the rest of the pixels will not be changed by this function. @end deftypefun @node Polygons, Qsort functions, Mesh grid for an image, Gnuastro library @subsection Polygons (@file{polygon.h}) Polygons are commonly necessary in image processing. In Gnuastro, they are used in ImageCrop (see @ref{ImageCrop}) for cutting out non-rectangular regions of a image. ImageWarp (see @ref{ImageWarp}) uses them to warp the images into a new pixel grid. The polygon related Gnuastro library macros and functions are introduced here. In all the functions here the vertices (and points) are defined as an array. So a polygon with 4 vertices will be identified with an array of 8 elements with the first two elements keeping the 2D coordinates of the first vertice and so on. @deffn Macro GAL_POLYGON_MAX_CORNERS The largest number of vertices a polygon can have in this library. @end deffn @deffn Macro GAL_POLYGON_ROUND_ERR @cindex Round-off error We have to consider floating point round-off errors when dealing with polygons. For example we will take @code{A} as the maximum of @code{A} and @code{B} when @code{A>B-GAL_POLYGON_ROUND_ERR}. @end deffn @deftypefun void gal_polygon_ordered_corners (double @code{*in}, size_t @code{n}, size_t @code{*ordinds}) We have a simple polygon (that can result from projection, so its edges don't collide or it doesn't have holes) and we want to order its corners in an anticlockwise fashion. This is necessary for clipping it and finding its area later. The input vertices can have practically any order. The input (@code{in}) is an array containing the coordinates (two values) of each vertice. @code{n} is the number of corners. So @code{in} should have @code{2*n} elements. The output (@code{ordinds}) is an array with @code{n} elements specifying the indexs in order. This array must have been allocated before calling this function. The indexes are output for more generic usage, for example in a homographic transform (necessary in warping an image, see @ref{Warping basics}), the necessary order of vertices is the same for all the pixels. In other words, only the positions of the vertices change, not the way they need to be ordered. Therefore, this function would only be necessary once. As a summary, the input is unchanged, only @code{n} values will be put in the @code{ordinds} array. Such that calling the input coordinates in the following fashion will give an anti-clockwise order when there are 4 vertices: @example 1st vertice: in[ordinds[0]*2], in[ordinds[0]*2+1] 2nd vertice: in[ordinds[1]*2], in[ordinds[1]*2+1] 3rd vertice: in[ordinds[2]*2], in[ordinds[2]*2+1] 4th vertice: in[ordinds[3]*2], in[ordinds[3]*2+1] @end example @cindex Convex Hull @noindent The implementation of this is very similar to the Graham scan in finding the Convex Hull. However, in projection we will never have a concave polygon (the left condition below, where this algorithm will get to E before D), we will always have a convex polygon (right case) or E won't exist! @example Concave Polygon Convex Polygon D --------C D------------- C \ | E / | \E | \ | / | \ | A--------B A ----------B @end example This is because we are always going to be calculating the area of the overlap between a quadrilateral and the pixel grid or the quadrilaterral its self. The @code{GAL_POLYGON_MAX_CORNERS} macro is defined so there will be no need to allocate these temporary arrays separately. Since we are dealing with pixels, the polygon can't really have too many vertices. @end deftypefun @deftypefun double gal_polygon_area (double @code{*v}, size_t @code{n}) Find the area of a polygon with vertices defined in @code{v}. @code{v} points to an array of doubles which keep the positions of the vertices such that @code{v[0]} and @code{v[1]} are the positions of the first vertice to be considered. @end deftypefun @deftypefun int gal_polygon_pin (double @code{*v}, double @code{*p}, size_t @code{n}) Return @code{1} if the point @code{p} is within the polygon whose vertices are defined by @code{v} and @code{0} otherwise. Note that the vertices of the polygon have to be sorted in an anti-clock-wise manner. @end deftypefun @deftypefun int gal_polygon_ppropin (double @code{*v}, double @code{*p}, size_t @code{n}) Similar to @code{gal_polygon_pin}, except that if the point @code{p} is on one of the edges of a polygon, this will return @code{0}. @end deftypefun @deftypefun void gal_polygon_clip (double @code{*s}, size_t @code{n}, double @code{*c}, size_t @code{m}, double @code{*o}, size_t @code{*numcrn}) Clip (find the overlap of) two polygons. This function uses the @url{https://en.wikipedia.org/wiki/Sutherland%E2%80%93Hodgman_algorithm, Sutherland-Hodgman} polygon clipping algorithm. Note that the vertices of both polygons have to be sorted in an anti-clock-wise manner. @end deftypefun @node Qsort functions, Spatial convolution, Polygons, Gnuastro library @subsection Qsort functions (@file{qsort.h}) The C programming language comes with the @code{qsort} (Quick sort) function. By allowing you to define the sorting based on the data, @code{qsort} is a generic function which allows you to sort any kind of data structure. The functions here are all meant to be passed onto @code{qsort} for sorting the respective types of data in the respective manner. Because of this all these functions have the same two argument types. @deffn {Global variable} {gal_qsort_index_arr} Pointer to a floating point array (@code{float *}) to use as a reference in @code{gal_qsort_index_float_decreasing}, see the explanation there for more. @end deffn @deftypefun int gal_qsort_int_decreasing (const void @code{*a}, const void @code{*b}) When passed to @code{qsort}, this function will sort an integer array in decreasing order. @end deftypefun @deftypefun int gal_qsort_int_increasing (const void @code{*a}, const void @code{*b}) When passed to @code{qsort}, this function will sort an integer array in increasing order. @end deftypefun @deftypefun int gal_qsort_float_decreasing (const void @code{*a}, const void @code{*b}) When passed to @code{qsort}, this function will sort a single precision floating point array in decreasing order. @end deftypefun @deftypefun int gal_qsort_float_increasing (const void @code{*a}, const void @code{*b}) When passed to @code{qsort}, this function will sort a single precision floating point array in increasing order. @end deftypefun @deftypefun int gal_qsort_double_decreasing (const void @code{*a}, const void @code{*b}) When passed to @code{qsort}, this function will sort a double precision floating point array in decreasing order. @end deftypefun @deftypefun int gal_qsort_double_increasing (const void @code{*a}, const void @code{*b}) When passed to @code{qsort}, this function will sort a double precision floating point array in increasing order. @end deftypefun @deftypefun int gal_qsort_index_float_decreasing (const void @code{*a}, const void @code{*b}) When passed to @code{qsort}, this function will sort a @code{size_t} array based on decreasing values in the @code{gal_qsort_index_arr} single precision floating point array. The floating point array will not be changed, it is only read. For example, if we have the following source code: @example #include #include /* qsort is defined in stdlib.h. */ #include int main (void) @{ size_t s[4]=@{0, 1, 2, 3@}; float f[4]=@{1.3,0.2,1.8,0.1@}; gal_qsort_index_arr=f; qsort(s, 4, sizeof(size_t), gal_qsort_index_float_decreasing); printf("%zu, %zu, %zu, %zu\n", s[0], s[1], s[2], s[3]); return EXIT_SUCCESS; @} @end example @noindent The output will be: @code{2, 0, 1, 3}. @end deftypefun @node Spatial convolution, Statistical operations, Qsort functions, Gnuastro library @subsection Spatial convolution (@file{spatialconvolve.h}) Convolution is a common operation in data processing and is fully explained in @ref{Spatial domain convolution} as part of @ref{Convolve}. We will therefore not explain the details, or its purpose here. The main high-level function here is @code{gal_spatialconvolve_convolve} which will do spatial convolution on multiple threads. The structure and functions introduced here are declared in @file{gnuastro/spatialconvolve.h}. In the first release of the Gnuastro libraries, this is the most high-level library since it was needed by multiple programs. In future releases this library will most probably merge with the frequency domain convolution functions to allow programmers to choose from the type of convolution they want. The main @deffn Structure gal_spatialconvolve_params This structure keeps all the basic convolution information so subsequent calls can be simpler. Please see the header for the details of its elements, complemented with comments. @end deffn @deftypefun void gal_spatialconvolve_pparams (float @code{*input}, size_t @code{is0}, size_t @code{is1}, float @code{*kernel}, size_t @code{ks0}, size_t @code{ks1}, size_t @code{nt}, int @code{edgecorrection}, float @code{*out}, size_t @code{*indexs}, struct gal_spatialconvolve_params @code{*scp}) Initialize @code{gal_spatialconvolve_params} with the given arguments. @end deftypefun @deftypefun {void *} gal_spatialconvolve_thread (void @code{*inparam}) This function should be passed onto @code{pthread_create} to create a new thread for convolution on a region of the image. @end deftypefun @deftypefun void gal_spatialconvolve_convolve (float @code{*input}, size_t @code{is0}, size_t @code{is1}, float @code{*kernel}, size_t @code{ks0}, size_t @code{ks1}, size_t @code{numthreads}, int @code{edgecorrection}, float @code{**out}) Convolve @code{input} (with @code{is0*is1} pixels) with the @code{kernel} (with @code{ks0*ks1}) on @code{numthreads} CPU threads. If you want edge-correction (see @ref{Edges in the spatial domain}), then set @code{edgecorrection} to @code{1}, otherwise set it to @code{0}. Memory will be allocated for the output and the convolved image will be stored in @code{out}. @end deftypefun @node Statistical operations, Multithreaded programming, Spatial convolution, Gnuastro library @subsection Statistical operations (@file{statistics.h}) This header includes a large variety of very basic statistical operators for various data types. Please note that we expect to greatly simplify the functions here for easier and more general usage in future releases. Ideally, they should be completely removed and the GNU Scientific Library's functions should be used. Since these functions are used in various parts of Gnuastro for multiple purposes, in this first library release (Gnuastro 0.2), there might be parallels, or non-homogeneous arguments. Such situations arise here because of the history of Gnuastro: the libraries grew out of the programs, so it will take a little while to correct. @deffn Structure GAL_STATISTICS_MAX_SIG_CLIP_CONVERGE The maximum number of times to try for @mymath{\sigma}-clipping (see @ref{Sigma clipping}). @end deffn @deftypefun void gal_statistics_long_non_blank_min (long @code{*in}, size_t @code{size}, long @code{*min}, long @code{blank}) Find the the minimum (non-blank) value in the @code{in} array (with @code{size} elements). The long type doesn't have a NaN value like the float types, see @ref{Blank pixels}. So as blank pixels, a value in the range of acceptable values (@code{blank} must be given so it is explicitly ignored. You can use @code{GAL_FITS_LONG_BLANK} in @file{gnuastro/fits.h}. @end deftypefun @deftypefun void gal_statistics_long_non_blank_max (long @code{*in}, size_t @code{size}, long @code{*max}, long @code{blank}) Similar to @code{gal_statistics_long_non_blank_min}, but find the maximum. @end deftypefun @deftypefun void gal_statistics_float_min (float @code{*in}, size_t @code{size}, float @code{*min}) Find the minimum value in the single precision floating point @code{in} array (with @code{size} elements) and store the value in @code{min}. Note that for all floating point types, any blank (NaN) value will be automatically ignored in this function. @end deftypefun @deftypefun void gal_statistics_float_max (float @code{*in}, size_t @code{size}, float @code{*max}) Similar to @code{gal_statistics_float_min} but find the maximum. @end deftypefun @deftypefun void gal_statistics_double_min (double @code{*in}, size_t @code{size}, double @code{*min}) Similar to @code{gal_statistics_float_min} but for double precision floating point types. @end deftypefun @deftypefun double gal_statistics_double_min_return (double @code{*in}, size_t @code{size}) Similar to @code{gal_statistics_double_min} but minimum will be returned, not put in a pointer. @end deftypefun @deftypefun void gal_statistics_double_max (double @code{*in}, size_t @code{size}, double @code{*max}) Similar to @code{gal_statistics_double_min}, but find maximum value. @end deftypefun @deftypefun double gal_statistics_double_max_return (double @code{*in}, size_t @code{size}) Similar to @code{gal_statistics_double_max_return}, but return maximum. @end deftypefun @deftypefun void gal_statistics_float_max_masked (float @code{*in}, unsigned char @code{*mask}, size_t @code{size}, float @code{*max}) Only find maximum where @code{mask} has a value of @code{0}. @end deftypefun @deftypefun void gal_statistics_float_second_max (float @code{*in}, size_t @code{size}, float @code{*secondmax}) Find the second largest value in the array. @end deftypefun @deftypefun void gal_statistics_float_second_min (float @code{*in}, size_t @code{size}, float @code{*secondmin}) Find the second smallest value in the array. @end deftypefun @deftypefun void gal_statistics_f_min_max (float @code{*in}, size_t @code{size}, float @code{*min}, float @code{*max}) Find the minimum and maximum simultaneously for single precision floating point types. @end deftypefun @deftypefun void gal_statistics_d_min_max (double @code{*in}, size_t @code{size}, double @code{*min}, double @code{*max}) Similar to @code{gal_statistics_f_min_max}, but for double precision floating point types. @end deftypefun @deftypefun void gal_statistics_f_max_with_index (float @code{*in}, size_t @code{size}, float @code{*max}, size_t @code{*index}) Find the maximum value in the array along with its index for a single precision floating point array. @end deftypefun @deftypefun void gal_statistics_d_max_with_index (double @code{*in}, size_t @code{size}, double @code{*max}, size_t @code{*index}) Similar to @code{gal_statistics_f_max_with_index}, but for a double precision floating point array. @end deftypefun @deftypefun void gal_statistics_d_min_with_index (double @code{*in}, size_t @code{size}, double @code{*min}, size_t @code{*index}) @end deftypefun @deftypefun void gal_statistics_f_min_with_index (float @code{*in}, size_t @code{size}, float @code{*min}, size_t @code{*index}) @end deftypefun @deftypefun float gal_statistics_float_sum (float @code{*in}, size_t @code{size}) Return the sum of the single precision floating point arrays. Note that NaN values will be ignored. @end deftypefun @deftypefun float gal_statistics_float_sum_num (float @code{*in}, size_t @code{*size}) Return the sum of elements in the floating point array along with the number of used (non-Nan) elements. @end deftypefun @deftypefun float gal_statistics_float_sum_squared (float @code{*in}, size_t @code{size}) Return the sum of squares of non-NaN elements in the array. @end deftypefun @deftypefun float gal_statistics_float_sum_mask (float @code{*in}, unsigned char @code{*mask}, size_t @code{size}, size_t @code{*nsize}) Given a mask (@code{mask}), return the sum of elements with a @code{mask} value of @code{0} (masked pixels are considered to have a non-zero value) and put the number of used elements in @code{nsize}. @end deftypefun @deftypefun float gal_statistics_float_sum_mask_l (float @code{*in}, long @code{*mask}, size_t @code{size}, size_t @code{*nsize}) Similar to @code{gal_statistics_float_sum_mask}, but when the mask is a long type. @end deftypefun @deftypefun float gal_statistics_float_sum_squared_mask (float @code{*in}, unsigned char @code{*mask}, size_t @code{size}, size_t @code{*nsize}) Return the sum of the squared elements in @code{in} that are not masked (corresponding element in @code{mask} is @code{0}. @end deftypefun @deftypefun float gal_statistics_float_sum_squared_mask_l (float @code{*in}, long @code{*mask}, size_t @code{size}, size_t @code{*nsize}) Similar to @code{gal_statistics_float_sum_squared_mask} but when the mask is a long type. @end deftypefun @deftypefun float gal_statistics_float_average (float @code{*in}, size_t @code{size}) Return the average of the single precision floating point array @code{in} with @code{size} elements. @end deftypefun @deftypefun double gal_statistics_double_average (double @code{*in}, size_t @code{size}) Return the average of the double precision floating point array @code{in} with @code{size} elements. @end deftypefun @deftypefun void gal_statistics_f_ave (float @code{*in}, size_t @code{size}, float @code{*ave}, unsigned char @code{*mask}) Return the average of the single precision floating point array @code{in} with @code{size} elements, do not use those elements where @code{mask} is non-zero. @end deftypefun @deftypefun void gal_statistics_f_ave_l (float @code{*in}, size_t @code{size}, float @code{*ave}, long @code{*mask}) Similar to @code{gal_statistics_f_ave}, but when the mask is of type long. @end deftypefun @deftypefun void gal_statistics_f_ave_std (float @code{*in}, size_t @code{size}, float @code{*ave}, float @code{*std}, unsigned char @code{*mask}) Find the average and standard deviation of the @code{in} array for pixels where @code{mask} has value of @code{0}. @end deftypefun @deftypefun void gal_statistics_f_ave_std_l (float @code{*in}, size_t @code{size}, float @code{*ave}, float @code{*std}, long @code{*mask}) Similar to @code{gal_statistics_f_ave_std}, but when the mask has a type of long. @end deftypefun @deftypefun float gal_statistics_median (float @code{*array}, size_t @code{insize}) Return the median value of a single precision floating point array @code{array} (which has @code{insize} elements). @end deftypefun @deftypefun double gal_statistics_median_double_in_place (double @code{*array}, size_t @code{insize}) Return the median value of a double precision floating point array @code{array} (which has @code{insize} elements). After this function, the elements of @code{array} are also sorted. @end deftypefun @deftypefun void gal_statistics_set_bins (float @code{*sorted}, size_t @code{size}, size_t @code{numbins}, float @code{min}, float @code{max}, float @code{onebinvalue}, float @code{quant}, float @code{**obins}) Given the input @code{sorted} array with @code{size} elements, a given number of @code{numbins}, an optional @code{min} and @code{max}, find the the bin starting points and keep them in @code{obins}. @code{obins} has two columns, and this function only fills the first column. The second will be filled by the histogram or cumulative distribution plots. If @code{onebinvalue} is NaN, then the bins above will be reported. However, if it is not NaN, all the bins will be shifted such that the lower value of one of the bins will be placed on this value of this variable (if it is in the range of the data). When @code{min==max}, the actual data range will be used. When @code{quant} is not zero (let's say it has the value @mymath{q}, for quantile) and @code{min==max} then the automatic range finder will use the values at the quantiles @mymath{q} and @mymath{1-q}. @end deftypefun @deftypefun void gal_statistics_histogram (float @code{*sorted}, size_t @code{size}, float @code{*bins}, size_t @code{numbins}, int @code{normhist}, int @code{maxhistone}) Build the histogram of the data (@code{sorted}, with @code{size} elements) in the @code{bins} array which also contains the starting bin values and has @code{numbins} rows. See @code{gal_statistics_set_bins}. When @code{normhist} is non-zero, the histogram will be normalized so the sum of all the bin values is unity. When @code{maxhistone} is non-zero, the histogram is scaled such that the bin with the largest value gets a value of 1. @end deftypefun @deftypefun void gal_statistics_cumulative_fp (float @code{*sorted}, size_t @code{size}, float @code{*bins}, size_t @code{numbins}, int @code{normcfp}) Build the cumulative frequency plot of the data (@code{sorted}, with @code{size} elements) in the @code{bins} array which also contains the starting bin values and has @code{numbins} rows. See @code{gal_statistics_set_bins}. When @code{normcfp} is non-zero, the cumulative frequency plot will be normalized so the last bin has a value of 1. @end deftypefun @deftypefun void gal_statistics_save_hist (float @code{*sorted}, size_t @code{size}, size_t @code{numbins}, char @code{*filename}, char @code{*comment}) Create a histogram of the data in @code{sorted} (and @code{size} elements) with @code{numbins} and save it into an ASCII text file named @file{filename} with a possible set of comments (pointed to by @code{comment} before he table. @end deftypefun @deftypefun size_t gal_statistics_index_from_quantile (size_t @code{size}, float @code{quant}) Given the number of elements (@code{size}), return the index corresponding to the quantile @code{quant}. @end deftypefun @deftypefun int gal_statistics_sigma_clip_converge (float @code{*array}, int @code{o1_n0}, size_t @code{num_elem}, float @code{sigma_multiple}, float @code{accuracy}, float @code{*outave}, float @code{*outmed}, float @code{*outstd}, int @code{print}) Calculate the @mymath{\sigma}-clipped (by convergence) average, median and standard deviation on the array @code{array} with @code{num_elem} elements (see @ref{Sigma clipping}). If @code{o1_n0==1}, then it is assumed that the input array is sorted. @code{sigma_multiple} is the multiple of @mymath{\sigma} used in the @mymath{\sigma}-clipping. If the @mymath{\sigma}-clipping did converge, then this function will return @code{0}, otherwise, it will return @code{1}. If @code{print} is non-zero, then the average, median and standard deviation of each step are printed. @end deftypefun @deftypefun int gal_statistics_sigma_clip_certain_num (float @code{*array}, int @code{o1_n0}, size_t @code{num_elem}, float @code{sigma_multiple}, size_t @code{numtimes}, float @code{*outave}, float @code{*outmed}, float @code{*outstd}, int @code{print}) Calculate the @mymath{\sigma}-clipped (with a fixed number of times) average, median and standard deviation on the array @code{array} with @code{num_elem} elements (see @ref{Sigma clipping}). If @code{o1_n0==1}, then it is assumed that the input array is sorted. @code{sigma_multiple} is the multiple of @mymath{\sigma} and @code{numtimes} is the number of times @mymath{\sigma}-clipping is done. If the @mymath{\sigma}-clipping was normally done, then this function will return @code{0}, otherwise, it will return @code{1}. If @code{print} is non-zero, then the average, median and standard deviation of each step are printed. @end deftypefun @deftypefun void gal_statistics_remove_outliers_flat_cdf (float @code{*sorted}, size_t @code{*outsize}) Remove the outliers in a distribution based on the slope of the cumulative frequency plot (when it becomes too flat). Before this function, @code{outssize} will point to the number of elements in @code{sorted}, after this function, it will be the number of elements that are not outliers. @end deftypefun @deffn Macro GAL_STATISTICS_MODE_LOW_QUANTILE The lower quantile used in calculating the mode. @end deffn @deffn Macro GAL_STATISTICS_MODE_HIGH_QUANTILE The lower quantile used in calculating the mode. @end deffn @deffn Macro GAL_STATISTICS_MODE_SYM_GOOD The acceptable value for the mode calculation symmetry. @end deffn @deffn Macro GAL_STATISTICS_MODE_LOW_QUANT_GOOD The lowest quantile that an acceptable mode can have. @end deffn @deffn Macro GAL_STATISTICS_MODE_SYMMETRICITY_LOW_QUANT Lower quantile for calculating the symmetricity. @end deffn @deffn Structure gal_statistics_mode_params The input parameters for the mode functions, this is mainly an internal structure and will become hidden in future releases. @end deffn @deftypefun void gal_statistics_mode_mirror_plots (float @code{*sorted}, size_t @code{size}, size_t @code{mirrorindex}, float @code{min}, float @code{max}, size_t @code{numbins}, char @code{*histsname}, char @code{*cfpsname}, float @code{mirrorplotdist}) Create a mirror plot based on the index given by @code{mirrorindex}. The mode calculation function procedure is defined in Appendix C of Akhlaghi and Ichikawa (2015, ApJS 220, 1. arXiv:1505.01664). @end deftypefun @deftypefun float gal_statistics_mode_value_from_sym (float @code{*sorted}, size_t @code{size}, size_t @code{modeindex}, float @code{sym}) It happens that you have the symmetricity and you want the flux value at that point, this function will do that job. The mode calculation function procedure is defined in Appendix C of Akhlaghi and Ichikawa (2015, ApJS 220, 1. arXiv:1505.01664). @end deftypefun @deftypefun void gal_statistics_mode_index_in_sorted (float @code{*sorted}, size_t @code{size}, float @code{errorstdm}, size_t @code{*modeindex}, float @code{*modesym}) Find the quantile of the mode of a sorted distribution. The return value is either @code{0} (not accurate) or @code{1} (accurate). The mode calculation function procedure is defined in Appendix C of Akhlaghi and Ichikawa (2015, ApJS 220, 1. arXiv:1505.01664). @end deftypefun @node Multithreaded programming, Text table into a C array, Statistical operations, Gnuastro library @subsection Multithreaded programming (@file{threads.h}) @cindex Multithreaded programming In modern times, newer CPU generations don't have significantly higher frequencies any more. However, CPUs are being manufactured with more cores, enabling more than one operation (thread) at each instant. This can be very useful to speed up many aspects of processing and in particular image processing. Most of the programs in Gnuastro utilize multi-threaded programming for the CPU intensive processing steps. This can potentially lead to a significant decrease in the running time of a program, see @ref{A note on threads}. In terms of reading the code, you don't need to know anything about multi-threaded programming. You can simply follow the case where only one thread is to be used. In these cases, threads are not used and can be completely ignored. @cindex POSIX threads library @cindex Lawrence Livermore National Laboratory At the time K&R's book was written, using threads was not common, so C's threading capabilities aren't introduced there. We use POSIX threads for multi-threaded programming, defined in the @file{pthread.h} system wide header. There are various resources for learning to use POSIX threads, the excellent tutorial from @url{https://computing.llnl.gov/tutorials/pthreads/, LLNL} is a very good start. The book `Advanced programming in the Unix environment'@footnote{Don't let the title scare you! The two chapters on Multi-threaded programming are very self-sufficient and don't need any more knowledge than K&R.}, by Richard Stevens and Stephen Rago, Addison-Wesley, 2013 (Third edition) also has two chapters explaining the POSIX thread constructs which can be very helpful. @cindex OpenMP An alternative to POSIX threads was OpenMP, but POSIX threads are low level, allowing much more control, while being easier to understand, see @ref{Why C}. All the situations where threads are used are completely independent with minimal need of coordination between the threads. Such problems are known as ``embarrassingly parallel'' problems. They are some of the simplest problems to solve with threads and also the ones that benefit most from threads, see the LLNL introduction@footnote{@url{https://computing.llnl.gov/tutorials/parallel_comp/}}. One very useful POSIX thread concept is @code{pthread_barrier}. Unfortunately, it is only an optional feature in the POSIX standard, so some operating systems don't include it. Therefore in @ref{Implementation of pthread_barrier}, we introduce our own implementation. You can ignore this section if your system has this construct. Following that, we describe the helper functions in this header that can greatly simplify writing a multi-threaded program, see @ref{Gnuastro's thread related functions} for more. @menu * Implementation of pthread_barrier:: Some systems don't have pthread_barrier * Gnuastro's thread related functions:: Functions for managing threads. @end menu @node Implementation of pthread_barrier, Gnuastro's thread related functions, Multithreaded programming, Multithreaded programming @subsubsection Implementation of @code{pthread_barrier} @cindex POSIX threads @cindex pthread_barrier One optional feature of the POSIX Threads standard is the @code{pthread_barrier} concept. It is a very useful high-level construct that allows for independent threads to ``wait'' behind a ``barrier'' for the rest after they finish. Barriers can thus greatly simplify the code in a multi-threaded program, so they are heavily used in Gnuastro. However, since its an optional feature in the POSIX standard, some operating systems don't include it. So to make Gnuastro portable, we have written our own implementation of those @code{pthread_barrier} functions. At @command{./configure} time, Gnuastro will check if @code{pthread_barrier} constructs are available on your system or not. If @code{pthread_barrier} is not available, our internal implementation will be compiled into the Gnuastro library and the definitions and declarations below will be usable in your code with @code{#include }. @deffn Type pthread_barrierattr_t Type to specify the attributes of a POSIX threads barrier. @end deffn @deffn Type pthread_barrier_t Structure defining the POSIX threads barrier. @end deffn @deftypefun int pthread_barrier_init (pthread_barrier_t @code{*b}, pthread_barrierattr_t @code{*attr}, unsigned int @code{limit}) Initialize the barrier @code{b}, with the attributes @code{attr} and total @code{limit} (a number of) threads that must wait behind it. This function must be called before spinning off threads. @end deftypefun @deftypefun int pthread_barrier_wait (pthread_barrier_t @code{*b}) This function is called within each thread, just before it is ready to return. Once a thread's function hits this, it will ``wait'' until all the other functions are also finished. @end deftypefun @deftypefun int pthread_barrier_destroy (pthread_barrier_t @code{*b}) Destroy all the information in the barrier structure. This should be called by the function that spinned-off the threads after all the threads have finished. @cartouche @noindent @strong{Destroy a barrier before re-using it:} It is very important to destroy the barrier before (possibly) reusing it. This destroy function not only destroys the internal structures, it also waits (in 1 microsecond intervals, so you will not notice!) until all the threads don't need the barrier structure any more. If you immediately start spinning off new threads with a not-destroyed barrier, then the internal structure of the remaining threads will get mixed with the new ones and you will get very strange and apparently random errors that are extremely hard to debug. @end cartouche @end deftypefun @node Gnuastro's thread related functions, , Implementation of pthread_barrier, Multithreaded programming @subsubsection Gnuastro's thread related functions These are some high-level functions in @file{gnuastro/threads.h} to facilitate programming in with POSIX threads. We have created a simple C program for testing these functions in @file{tests/lib/multithread.c}. This small program was compiled and run on your system when you ran @command{make check}. You can use it as a template to easily create small multi-threaded programs and efficiently use your powerful CPU. @deffn Macro GAL_THREADS_NON_THRD_INDEX This value will be used in the output of @code{gal_threads_dist_in_threads} as a non-index. It plays the same role as a string's null character: `@code{\0}': as soon as the parser sees this value, it will stop continuing. @end deffn @deftypefun void gal_threads_attr_barrier_init (pthread_attr_t @code{*attr}, pthread_barrier_t @code{*b}, size_t @code{limit}) @cindex Detached threads Initialize the general thread attribute @code{attr} and the barrier @code{b} with @code{limit} threads to wait behind the barrier. For maximum efficiency, the threads initialized with this function will be detached. Therefore no communication is possible between these threads and in particular @code{pthread_join} won't work on these threads. You have to use the barrier constructs to wait for all threads to finish. @end deftypefun @deftypefun void gal_threads_dist_in_threads (size_t @code{numactions}, size_t @code{numthreads}, size_t @code{**outthrds}, size_t @code{*outthrdcols}) Identify the ``index''es (starting from 0) of the actions to be done on each thread in the @code{outthrds} array. @code{outthrds} is treated as a 2D array with @code{numthreads} rows and @code{outthrdcols} columns. The indexs in each row, identify the actions that should be done by one thread. Please see the explanation below to understand the purpose of this operation. Let's assume you have @mymath{A} actions (where there is only one function and the input values differ for each action) and @mymath{T} threads available to the system with @mymath{A>T} (common values for these two would be @mymath{A>1000} and @mymath{T<10}). Spinning off a thread is not a cheap job and requires a significant number of CPU cycles. Therefore, creating @mymath{A} threads is not the best way to address such a problem. The most efficient way to manage the actions is such that only @mymath{T} threads are created, and each thread works on a list of actions identified for it in series (one after the other). This way your CPU will get all the actions done with minimal overhead. The purpose of this function is to do do what we explained above: each row in the @code{outthrds} array contains the indexs of actions which must be done by one thread. @code{outthrds} contains @code{outthrdcols} columns. In using @code{outthrds}, you don't have to know the number of columns. The @code{GAL_THREADS_NON_THRD_INDEX} macro has a role very similar to a string's @code{\0}: every row finishes with this macro, so can easily stop parsing the indexes in the row when you confront it. Please see the example program in @file{tests/lib/multithread.c} for a demonstration. @end deftypefun @node Text table into a C array, World Coordinate System, Multithreaded programming, Gnuastro library @subsection Text table into a C array (@file{txtarray.h}) One of the most common formats to store and transfer normally sized data are ASCII files (which can be seen on a text editor). During your processing experiments (with the data, or what programmers call ``developing'') you will also often want to see how your data is being processed and one of the easiest ways to check out your arrays is to write them out as an ASCII file and check them. The functions here are mainly focused on tables that contain numbers. @deffn Macro GAL_TXTARRAY_LOG When an element of the input table cannot be read as a number, the column and row number of the element are stored along with the element into one row of a log file. This macro contains the name of the log-file. @end deffn @deftypefun void gal_txtarray_txt_to_array (char @code{*filename}, double @code{**array}, size_t @code{*s0}, size_t @code{*s1}) Store the ASCII text table in @file{filename} into the C array @code{array} which has @code{s0} rows and @code{s1} columns. Any blank lines or lines starting with @code{#} (comments) will be ignored. The column delimiters (separating one column from the previous and next) are `@code{ }' (space), `@code{,}', `TAB'. @end deftypefun @deftypefun void gal_txtarray_printf_format (int @code{numcols}, char @code{**fmt}, int @code{*int_cols}, int @code{*accu_cols}, int @code{*space}, int @code{*prec}, char @code{forg}) Return the @code{printf} formatting string (@code{fmt}) for @code{numcols} columns. Three types of output columns are assumed: integers, normal accuracy floating points and extra-precision floating points. Normally most columns will not need too much accuracy when printing (for example only 3 decimals might be enough). However usually a very limited number of columns will need more precision (like RA and Dec). So to store space (each character is a byte) and also make the table more readable, we allow these two types of floating points. @code{int_cols} and @code{accu_cols} are arrays containing the column numbers (starting from zero) that contain integers and extra-accuracy columns. The ending of the column indexes in @code{int_cols} and @code{accu_cols} is defined by a negative number. @code{space} is a three element array which will keep the number of characters that must be used for the integer, normal-accuracy and extra-accuracy columns. @code{prec} is a two element array which contains the number of decimals to print for the normal and extra accuracy columns. @code{forg} (read as `f-or-g') is the @code{printf} type for the floating point numbers: either @code{f} (as in @code{%f}, which will only print decimals) and @code{g} (as in @code{%g}, for either printing decimals or exponentials). See @code{gal_txtarray_array_to_txt} for more. @end deftypefun @deftypefun void gal_txtarray_array_to_txt (double @code{*array}, size_t @code{s0}, size_t @code{s1}, char @code{*comments}, int @code{*int_cols}, int @code{*accu_cols}, int @code{*space}, int @code{*prec}, char @code{forg}, const char @code{*filename}) Print the C array @code{array} (with @code{s0} rows and @code{s1} columns) as an ASCII text table in @code{filename}. The string pointed to by @code{comments} will be printed at the top of the table. See the explanation of @code{gal_txtarray_printf_format} for the other arguments. @end deftypefun @node World Coordinate System, , Text table into a C array, Gnuastro library @subsection World Coordinate System (@file{wcs.h}) The FITS world coordinate system is a mechanism to give physical values to the data points. In the case of images, it can be used to convert pixel images to celestial coordinates like the right ascension and declination. Gnuastro doesn't have any functions to actually do the transformations, the standard tool for doing this in astronomy is WCSLIB (see @ref{WCSLIB}). The functions introduced here are just wrappers around the lower-level functions provided by WCSLIB. @deftypefun void gal_wcs_xy_array_to_radec (struct wcsprm @code{*wcs}, double @code{*xy}, double @code{*radec}, size_t @code{number}, size_t @code{stride}) Convert the image coordinates @code{xy} (a two column array with @code{number} rows) to world coordinates @code{wcs} (also a two column array, which has to have been allocated prior to this function) using the conversion parameters in @code{wcs}. @code{stride} is the number of columns in a larger array, see below. It might happen that you have one array which contains both the image and world coordinates along with many more columns. @code{stride} is the width of that larger array. If such an array doesn't exist and @code{xy} and @code{radec} are separately allocated arrays with @mymath{2\times}@code{number} elements, then just set the value of @code{stride} to @code{2}. @end deftypefun @deftypefun void gal_wcs_radec_array_to_xy (struct wcsprm @code{*wcs}, double @code{*radec}, double @code{*xy}, size_t @code{number}, size_t @code{stride}) Similar to @code{gal_wcs_xy_array_to_radec} but convert the world coordinates in @code{radec} to image coordinates in @code{xy}. @end deftypefun @deftypefun double gal_wcs_angular_distance_deg (double @code{r1}, double @code{d1}, double @code{r2}, double @code{d2}) Return the angular distance (in degrees) between a point located at (@code{r1}, @code{d1}) to (@code{r2}, @code{d2}). All input coordinates are in degrees. The distance (along a great circle) on a sphere between two points is calculated with the equation below. Since the pixel sides are usually very small, we won't be using the direct formula: @dispmath {\cos(d)=\sin(d_1)\sin(d_2)+\cos(d_1)\cos(d_2)\cos(r_1-r_2)} Here, we will be using the @url{https://en.wikipedia.org/wiki/Haversine_formula, Haversine formula} which is better considering floating point errors: @dispmath{{\sin^2(d)\over 2}=\sin^2\left( {d_1-d_2\over 2} \right)+\cos(d_1)\cos(d_2)\sin^2\left( {r_1-r_2\over 2} \right)} @end deftypefun @deftypefun void gal_wcs_pixel_scale_deg (struct wcsprm @code{*wcs}, double @code{*dx}, double @code{*dy}) Return the pixel scale of the WCS structure @code{wcs} for the two image dimensions @code{dx} and @code{dy} in degrees. Here, the X-axis is the first FITS axis, or the horizontal axis when viewed in SAO ds9. @end deftypefun @deftypefun double gal_wcs_pixel_area_arcsec2 (struct wcsprm @code{*wcs}) Given the WCS structure @code{wcs} calculate the pixel area in arcsec-squared. @end deftypefun @node Developing, Gnuastro programs list, Libraries, Top @chapter Developing The basic idea of GNU Astronomy Utilities is for an interested astronomer to be able to easily understand the code of any of the programs or libraries, be able to modify the code if s/he feels there is an improvement and finally, to be able to add new programs or libraries for their own benefit, and the larger community if they are willing to share it. In short, we hope that at least from the software point of view, the ``obscurantist faith in the expert's special skill and in his personal knowledge and authority'' can be broken, see @ref{Science and its tools}. The following software architecture can be one of the most basic and easy to understand for any interested inquirer. In this chapter, first some general design choices are tackled in @code{Why C} and @code{Program design philosophy}. The project management webpage and mailing lists are explained in @ref{Gnuastro project webpage} and @code{Developing mailing lists}. In @ref{Coding conventions}, Gnuastro's adopted coding conventions are discussed and is followed by @ref{Program source} which describes how to easily navigate the source files in each program and also contains a template program to easily add new programs. Some other general aspects are then discussed: @ref{Documentation}, @ref{Building and debugging}, @ref{Test scripts}, and @ref{Developer's checklist}. This chapter finishes with a full description of Gnuastro's work-flow in @ref{Contributing to Gnuastro}. @menu * Why C:: Why Gnuastro is designed in C. * Program design philosophy:: General ideas behind the package structure. * Gnuastro project webpage:: Central hub for Gnuastro activities. * Developing mailing lists:: Stay up to date with Gnuastro's development. * Coding conventions:: Gnuastro coding conventions. * Program source:: Conventions for the code. * Documentation:: Documentation is an integral part of Gnuastro. * Building and debugging:: Build and possibly debug during development. * Test scripts:: Understanding the test scripts. * Developer's checklist:: Checklist to finalize your changes. * Contributing to Gnuastro:: Share your changes with all users. @end menu @node Why C, Program design philosophy, Developing, Developing @section Why C programming language? @cindex C programming language @cindex C++ programming language @cindex Python programming language Currently the programming language that is most commonly used in scientific applications is C++, and more recently Python. One of the main reasons behind this choice is that through the Object oriented programming paradigm, they offer a much higher level of abstraction. However, GNU Astronomy Utilities are written in the C programming language. The reasons can be summarized with simplicity, portability and speed. All three are very important in a scientific software. @cindex ANSI C @cindex ISO C90 @cindex Ritchie, Dennis @cindex Kernighan, Brian @cindex Stroustrup, Bjarne Simplicity can best be demonstrated in a comparison of the main books of C++ and C. The ``C programming language''@footnote{Brian Kernighan, Dennis Ritchie. @emph{The C programming language}. Prentice Hall, Inc., Second edition, 1988. It is also commonly known as K&R and is based on the ANSI C and ISO C90 standards.} book, written by the authors of C, is only 286 pages and covers a very good fraction of the language, it has also remained unchanged from 1988. C is the main programming language of nearly all operating systems and there is no plan of any significant update. On the other hand, the most recent ``C++ programming language''@footnote{Bjarne Stroustrup. @emph{The C++ programming language}. Addison-Wesley Professional; 4 edition, 2013.} book, also written by its author, has 1366 pages and its fourth edition came out in 2013! As discussed in @ref{Science and its tools}, it is very important for other scientists to be able to readily read the code of a program at their will with minimum requirements. @cindex Object oriented programming In C++, inheriting objects in the object oriented programming paradigm and their internal functions make the code very easy to write for the programmer who is deeply invested in those objects and understands all their relations well. But it simultaneously makes reading the program for a first time reader (a curious scientist who wants to know only how a small step was done) extremely hard. Before understanding the methods, the scientist has to invest a lot of time in understanding those objects and their relations. But in C all variables can be given as the basic language types for example @code{int}s or @code{float}s and their pointers to define arrays. So when an outside reader is only interested in one part of the program, that part is all they have to understand. Recently it is also becoming common to write scientific software in Python, or a combination of it with C or C++. Python is a high level scripting language which doesn't need compilation. It is very useful when you want to do something on the go and don't want to be halted by the troubles of compiling, linking, memory checking, etc. When the data sets are small and the job is temporary, this ability of Python is great and is highly encouraged. A very good example might be plotting, in which Python is undoubtedly one of the best. But as the data sets increase in size and the processing becomes very complicated, the speed of Python scripts significantly decrease. So when the program doesn't change too often and is widely used in a large community mostly on large data sets (like astronomical images), using Python will waste a lot of valuable research-hours. It is possible to wrap C or C++ functions with Python to fix the speed issue. Like C++, Python is object oriented, so as explained above, it needs a high level of experience with that particular program to fully understand its inner workings. To make things worse, since it is mainly for fast and on the go programming, it can undergo significant changes. One recent example is how Python 2.x and Python 3.x are not compatible. Lots of research teams that invested heavily in Python 2.x cannot benefit from Python 3.x or future versions any more. Some converters are available, but since they are automatic, lots of complications might arise in the conversion. Thus, re-writing all the changes would be the only truly reliable option. If a research project begins using Python 3.x today, there is no telling how compatible their investments will be when Python 4.x or 5.x will come out. This stems from the core principles of Python, which are very useful when you look in the `on the go' basis as described before and not future usage. Future-proof code (as long as current operating systems will be used) will be written in C. The portability of C is best demonstrated by the fact that both C++ and Python are part of the C-family of programming languages which also include Java, Perl, and many other languages. C libraries can be immediately included in C++ and with it is easily possible to write wrappers for C libraries in programs in all C-family programming languages. This will allow other scientists to benefit from C libraries with any of those languages. With version 0.2, Gnuastro's C library is installed along with the programs and task 13786@footnote{@url{http://savannah.gnu.org/task/?13786}} has been defined to add wrappers for higher level languages. @cindex Low level programming @cindex Programming, low level The final reason was speed. This is another very important aspect of C which is not independent of simplicity (first reason discussed above). The abstractions provided by the higher-level languages (which also makes learning them harder for a newcomer) comes at the cost of speed. Since C is a low-level language@footnote{Low-level languages are those that directly operate the hardware like assembly languages. So C is actually a high-level language, but it can be considered one of the lowest-level, high-level languages.} (closer to the hardware), it is much less complex for both the human reader and the computer. The former was discussed above in simplicity and the latter helps in making the program run more efficiently (faster). This thus allows for a closer relation between the scientist/programmer (program) and the actual data/processing. The GNU coding standards@footnote{@url{http://www.gnu.org/prep/standards/}} also encourage the use of C over all other languages when generality of usage and ``high speed'' is desired. @node Program design philosophy, Gnuastro project webpage, Why C, Developing @section Program design philosophy The core processing functions of each program are written mostly with the basic ISO C90 standard. We do make lots of use of the GNU additions to the C language in the GNU C library, but these additional functions are mainly used in the user interface functions (reading your inputs and preparing them prior to or after the analysis). The actual algorithms, which most scientists would be more interested in, are much more closer to ISO C90. For this reason, the source files containing user interface code and those containing actual processing code are clearly separated, see @ref{Program source}. If anything particular to the GNU C library is used in the processing functions, it is explained in the comments in between the code. @cindex GNU Coreutils Similar to GNU Coreutils, all the Gnuastro programs provide very low level operations. This enables you to use the GNU Bash scripting language (which is the default in most GNU/Linux operating systems) or any other shell you might be using to operate on a large number of files or do very complex things through the creative combinations of these tools that the authors had never dreamed of. We have put a few simple examples in @ref{Tutorials}. @cindex GNU Bash @cindex Python Matplotlib @cindex Matplotlib, Python @cindex PGFplots in @TeX{} or @LaTeX{} For example all the analysis output is provided as ASCII tables which you can feed into your favorite plotting program to inspect visually. Python's Matplotlib is very useful for fast plotting of the tables to immediately check your results. If you want to include the plots in a document, you can use the PGFplots package within @LaTeX{}, no attempt is made to include such operations in Gnuastro. In short, Bash can act as a glue to connect the inputs and outputs of all these various Gnuastro programs (and other programs) in any fashion you please. The advantage of this architecture is that the programs become small and transparent: the starting and finishing point of every program is clearly demarcated. For nearly all operations on a modern computer, the read/write speed is very insignificant compared to the actual processing a program does. Therefore the complexity which arises from sharing memory in a large application is simply not worth the speed gain. This basic design is influenced by Eric Raymond's ``The Art of Unix Programming''@footnote{Eric S. Raymond, 2004, @emph{The Art of Unix Programming}, Addison-Wesley Professional Computing Series.} which beautifully describes the design philosophy and practice which lead to the success of Unix-based operating systems@footnote{KISS principle: Keep It Simple, Stupid!}. @node Gnuastro project webpage, Developing mailing lists, Program design philosophy, Developing @section Gnuastro project webpage @cindex Bug @cindex Issue @cindex Tracker @cindex Report a bug @cindex Management hub @cindex Feature request @cindex Central management @url{https://savannah.gnu.org/projects/gnuastro/, Gnuastro's central management hub}@footnote{@url{https://savannah.gnu.org/projects/gnuastro/}} is located on @url{https://savannah.gnu.org/, GNU Savannah}@footnote{@url{https://savannah.gnu.org/}}. It is the central software development management system for all GNU projects. Through this central hub, you can view the list of activities that the developers are engaged in, their activity on the version controlled source, and other things. Each defined activity in the development cycle is known as an `issue' (or `item'). An issue can be a bug (see @ref{Report a bug}), or a suggested feature (see @ref{Suggest new feature}) or an enhancement or generally any @emph{one} job that is to be done. In Savannah, issues are classified into three categories or `tracker's: @table @asis @cindex Mailing list: bug-gnuastro @item Support This tracker is a way that (possibly anonymous) users can get in touch with the Gnuastro developers. It is a complement to the bug-gnuastro mailing list (see @ref{Report a bug}). Anyone can post an issue to this tracker. The developers will not submit an issue to this list. They will only reassign the issues in this list to the other two trackers if they are valid@footnote{Some of the issues registered here might be due to a mistake on the user's side, not an actual bug in the program.}. Ideally (when the developers have time to put on Gnuastro, please don't forget that Gnuastro is a volunteer effort), there should be no open items in this tracker. @item Bugs This tracker contains all the known bugs in Gnuastro (problems with the existing tools). @item Tasks The items in this tracker contain the future plans (or new features/capabilities) that are to be added to Gnuastro. @end table @noindent All the trackers can be browsed by a (possibly anonymous) visitor, but to edit and comment on the Bugs and Tasks trackers, you have to be a registered Gnuastro developer. When posting an issue to a tracker, it is very important to choose the `Category' and `Item Group' options accurately. The first contains a list of all Gnuastro's programs along with `Installation', `New program' and `Webpage'. The ``Item Group'' contains the nature of the issue, for example if it is a `Crash' in the software (a bug), or a problem in the documentation (also a bug) or a feature request or an enhancement. The set of horizontal links on the top of the page (Starting with `Main' and `Homepage' and finishing with `News') are the easiest way to access these trackers (and other major aspects of the project) from any part of the project webpage. Hovering your mouse over them will open a drop down menu that will link you to the different things you can do on each tracker (for example, `Submit new' or `Browse'). When you browse each tracker, you can use the ``Display Criteria'' link above the list to limit the displayed issues to what you are interested in. The `Category' and `Group Item' (explained above) are a good starting point. @cindex Mailing list: gnuastro-devel Any new issue that is submitted to any of the trackers, or any comments that are posted for an issue, is directly forwarded to the gnuastro-devel mailing list (@url{https://lists.gnu.org/mailman/listinfo/gnuastro-devel}, see @ref{Developing mailing lists} for more). This will allow anyone interested to be up to date on the over-all development activity in Gnuastro and will also provide an alternative (to Savannah) archiving for the development discussions. Therefore, it is not recommended to directly post an email to this mailing list, but do all the activities (for example add new issues, or comment on existing ones) on Savannah. @cartouche @noindent @strong{Do I need to be a member in Savannah to contribute to Gnuastro?} No. The full version controlled history of Gnuastro is available for anonymous download or cloning. See @ref{Production workflow} for a description of Gnuastro's Integration-Manager Workflow. In short, you can either send in patches, or make your own fork. If you choose the latter, you can push your changes to your own fork and inform us. We will then pull your changes and merge them into the main project. Please see @ref{Forking tutorial} for a tutorial. @end cartouche @node Developing mailing lists, Coding conventions, Gnuastro project webpage, Developing @section Developing mailing lists To keep the developers and interested users up to date with the activity and discussions within Gnuastro, there are two mailing lists which you can subscribe to: @table @asis @item @command{gnuastro-devel@@gnu.org} @itemx (at @url{https://lists.gnu.org/mailman/listinfo/gnuastro-devel}) @cindex Mailing list: gnuastro-devel All the posts made in the support, bugs and tasks discussions of @ref{Gnuastro project webpage} are also sent to this mailing address and archived. By subscribing to this list you can stay up to date with the discussions that are going on between the developers before, during and (possibly) after working on an issue. All discussions are either in the context of bugs or tasks which are done on Savannah and circulated to all interested people through this mailing list. Therefore it is not recommended to post anything directly to this mailing list. Any mail that is sent to it from Savannah to this list has a link under the title ``Reply to this item at:''. That link will take you directly to the issue discussion page, where you can read the discussion history or join it. While you are posting comments on the Savannah issues, be sure to update the meta-data. For example if the task/bug is not assigned to anyone and you would like to take it, change the ``Assigned to'' box, or if you want to report that it has been applied, change the status and so on. All these changes will also be circulated with the email very clearly. @item @command{gnuastro-commits@@gnu.org} @itemx (at @url{https://lists.gnu.org/mailman/listinfo/gnuastro-commits}) @cindex Mailing list: gnuastro-commits This mailing list is defined to circulate all commits that are done in Gnuastro's version controlled source, see @ref{Version controlled source}. If you have any ideas, or suggestions on the commits, please use the bug and task trackers on Savannah to followup the discussion, do not post to this list. All the commits that are made for an already defined issue or task will state the respective ID so you can find it easily. @end table @node Coding conventions, Program source, Developing mailing lists, Developing @section Coding conventions @cindex GNU coding standards @cindex Gnuastro coding convention Generally we try our best to follow the GNU coding standards, besides those the following conventions are adhered to until now. If new code is also added in the same manner, it would be much more easily readable by any interested astronomer (who will become familiar with it after reading once). @itemize @item It is very important that the code be easy to read by the eye. So when the order of several lines within a function does not matter (mostly when defining variables at the start of a function). You should put the lines in the order of increasing length and group the variables with similar types such that this half-pyramid of declarations becomes most visible. If the reader is interested, a simple search will show them the variable they are interested in. However, when looking through the functions or reading the separate steps of the functions, this `order' in the declarations will make reading the rest of the function steps much more easier and pleasant to the eye. @item When ever you see that the function cannot be fully displayed (vertically) in your monitor, this is a sign that it has become too long and should be broken up into multiple functions. 40 lines is usually a good reference. When the start and end of a function are clearly visible in one glance, the function is much more easier to understand. This is most important for low-level functions (which usually define a lot of variables). Low-level functions do most of the processing, they will also be the most interesting part of a program for an inquiring astronomer. This convention is less important for higher level functions that don't define too many variables and whose only purpose is to run the lower-level functions in a specific order and with checks. @cindex Optimization flag @cindex GNU Compiler Collection In general you can be very liberal in breaking up the functions into smaller parts, the GNU Compiler Collection (GCC) will automatically compile the functions as inline functions when the optimizations are turned on. So you don't have to worry about decreasing the speed. By default Gnuastro will compile with the @option{-O3} optimization flag. @cindex Buffers (Emacs) @cindex Emacs buffers @item All Gnuastro hand-written text files (C source code, Texinfo documentation source, and version control commit messages) should not exceed @strong{75} characters per line. Monitors today are certainly much wider, but with this limit, reading the functions becomes much more easier. Also for the developers, it allows multiple files (or multiple views of one file) to be displayed beside each other on wide monitors. Emacs's buffers are excellent for this capability, setting a buffer width of 80 with `@key{C-u 80 C-x 3}' will allow you to view and work on several files or different parts of one file using the wide monitors common today. Emacs buffers can also be used as a shell prompt and compile the program (with @key{M-x compile}), and 80 characters is the default width in most terminal emulators. If you use Emacs, Gnuastro sets the 75 character @command{fill-column} variable automatically for you, see cartouche below. For long comments you can use press @key{Alt-q} in Emacs to separate them into separate lines automatically. For long literal strings, you can use the fact that in C, two strings immediately after each other are concatenated, for example @code{"The first part, " "and the second part."} Note the space character in the end of the first part. Since they are now separated, you can easily break a long literal string into several lines and adhere to the maximum 75 character line length policy. @cindex Header file @item The headers required by each source file (ending with @file{.c}) should be defined inside of it. All the headers a program needs should not be stacked in another header to include in all source files (for example @file{main.h}). Although most `professional' programmers choose the latter type, Gnuastro is primarily written for inquisitive astronomers (who are generally amateur programmers). This is very useful for readability by a first time reader. @file{main.h} may only include the header file(s) that define types that the main program structure needs, see @file{main.h} in @ref{Program source}. Those particular header files that are included in @file{main.h} can of course be ignored (not included) in separate source files. @item The headers should be classified (by an empty line) into separate groups: @enumerate @cindex Gnulib: GNU Portability Library @cindex GNU Portability Library (Gnulib) @item @code{#include }: This must be the first code line (not commented or blank) in each source file. It sets macros that the GNU Portability Library (Gnulib) will use for the possible additions/modifications to C library headers. @cindex GNU C library @item The C library (or GNU C library) header files, for example @file{stdio.h} or @file{errno.h}. @item Installed library header files, including Gnuastro's installed headers (for example @file{cfitsio.h} or @file{gsl/gsl_rng.h}, or @file{gnuastro/fits.h}). @item Gnuastro's internal headers (that are not installed), for example @file{commonparams.h}, or Gnulib's headers (which are also not installed) like @file{nproc.h}. @item For programs, the @file{main.h} file (which is needed by the next group of headers). @item That particular program's header files, for example @file{mkprof.h}, or @file{noisechisel.h}. @end enumerate @noindent As much as order does not matter when you include the header of each group, sort them by length, see above. @item All function names, variables, etc should be in lower case. Macros and pre-processor variables should be in upper case. @item Regarding naming of exported header files, functions, variables, macros, and library functions, we adopted similar conventions to those used by the GNU Scientific Library (GSL)@footnote{@url{https://www.gnu.org/software/gsl/design/gsl-design.html#SEC15}}. In particular, in order to avoid clashes with the names of functions and variables coming from other libraries the name-space `@code{gal_}' is prefixed to them. GAL stands for @emph{G}NU @emph{A}stronomy @emph{L}ibrary. Ideally `@code{gnuastro_}' should have been used, but that is very long. @item All installed header files should be in the @file{lib/gnuastro} directory (under the top Gnuastro source directory). After installation, they will be put in the @file{$prefix/include/gnuastro} directory (see @ref{Installation directory} for @file{$prefix}). Therefore with this convention Gnuastro's headers can be included in internal (to Gnuastro) and external (a library user) source files with the same line @example # include @end example Note that unlike the GSL convention, the header file names are not prefixed with a `@file{gal_}'. If a user manually mixes the Gnuastro (or GSL) headers with other headers, compilation will break because the installed headers depend on each other (the @code{#include} directive, with the @file{gnuastro/} directory, above is present in the installed headers too). Therefore the `@file{gal_}' prefix to the file names is redundant@footnote{Note that this applies to GSL's header files too, for example see @file{eigen/gsl_eigen.h} in GSL's source files. GSL uses the @file{gsl_} filename prefix to separate the headers that will be installed from those that won't. Therefore this filename prefix a technical internal issue there, which we believe will only confuse the user who doesn't need to get involved with such issues.}. @item @cindex GNU coding standards All installed functions and variables should also include the base name of the file in which they are defined as prefix, using underscores to separate words@footnote{The convention to use underscores to separate words, called ``snake case'' (or ``snake_case''). This is also recommended by the GNU coding standards.}. The same applies to exported macros, but in upper case. For example in Gnuastro's top source directory, the prototype of function @code{gal_box_border_from_center} is in @file{lib/gnuastro/box.h}, and the macro @code{GAL_POLYGON_MAX_CORNERS} is defined in @code{lib/gnuastro/polygon.h}. To find the header file in the installed directories, replace @file{lib/} with @file{$prefix/include/} (see @ref{Installation directory} for @file{$prefix}). This is necessary to give any user (who is not familiar with the library structure) the ability to follow the code of a function that is not in the program or library they are reading. This convention does make the function names longer (a little harder to write), but the extra documentation it provides convention plays an important role in Gnuastro and is worth the cost. @item @cindex GNU Emacs @cindex Trailing space There should be no trailing white space in a line. To do this automatically every time you save a file in Emacs, add the following line to your @file{~/.emacs} file. @example (add-hook 'before-save-hook 'delete-trailing-whitespace) @end example @item @cindex Tabs are evil There should be no tabs in the indentation@footnote{If you use Emacs, Gnuastro's @file{.dir-locals.el} file will automatically never use tabs for indentation. To make this a default in all your Emacs sessions, you can add the following line to your @file{~/.emacs} file: @command{(setq-default indent-tabs-mode nil)}}. @item @cindex GNU Emacs @cindex Function groups @cindex Groups of similar functions All similar functions are separated by 5 blank lines to be easily seen to be related in a group when parsing the source code by eye. In Emacs you can use @key{CTRL-u 5 CTRL-o}. @item One group of functions is separated from another with 20 blank lines. In Emacs you can use @key{CTRL-u 20 CTRL-o}. Each group of functions has short descriptive title of the functions in that group. This title is surrounded by asterisks (@key{*}) to make it clearly distinguishable. Such contextual grouping and clear title are very important for easily understanding the code. @end itemize The last two conventions are not common and might benefit from a short discussion here. With a good experience in advanced text editor operations, to some extent the last two are redundant for a professional developer. However, recall that Gnuastro aspires to be friendly to un-familiar, and un-experienced (in programming) eyes. In other words, as discussed in @ref{Science and its tools}, we want the code to appear welcoming to someone who is completely new to coding and only has a scientific curiosity. Newcomers to coding and development, who are curious enough to venture into the code, will not be using (or have any knowledge of) advanced text editors. They will see the raw code in the webpage or on a simple text editor (like Gedit) as plain text. Trying to learn and understand a file with dense functions that are all spaced with one or two blank lines can be very taunting for a newcomer. But when they scroll through the file and see clear titles and meaningful spaces for similar functions (less, meaningful density), we are helping them find and focus on the part they are most interested in sooner and easier. @cartouche @cindex GNU Emacs @noindent @strong{GNU Emacs, the recommended text editor:} GNU Emacs is an extensible and easily customizable text editor which many programmers rely on for developing due to its countless features. Among them, it allows specification of certain settings that are applied to a single file or to all files in a directory and its sub-directories. In order to harmonize code coming from different contributors, Gnuastro comes with a @file{.dir-locals.el} file which automatically configures Emacs to satisfy most of the coding conventions above when you are using it within Gnuastro's directories. Thus, Emacs users can readily start hacking into Gnuastro. If you are new to developing, we strongly recommend this editor. Emacs was the first project released by GNU and is still one of its flagship projects. Some resources can be found at: @table @asis @item Official manual At @url{https://www.gnu.org/software/emacs/manual/emacs.html}. This is a great and very complete manual which is being improved for over 30 years and is the best starting point to learn it. It just requires a little patience and practice, but rest assured that you will be rewarded. If you install Emacs, you also have access to this manual on the command-line with the following command (see @ref{Info}). @example $ info emacs @end example @item A guided tour of emacs At @url{https://www.gnu.org/software/emacs/tour/}. A short visual tour of Emacs, officially maintained by the Emacs developers. @item Unofficial mini-manual At @url{https://tuhdo.github.io/emacs-tutor.html}. A shorter manual which contains nice animated images of using Emacs. @end table @end cartouche @node Program source, Documentation, Coding conventions, Developing @section Program source @cindex Source file navigation @cindex Navigating source files @cindex Program structure convention @cindex Convention for program source @cindex Gnuastro program structure convention Besides the fact that all the programs share some functions that were explained in @ref{Libraries}, everything else about each program is completely independent. In this section the conventions used in all the program sources are explained in @ref{Mandatory source code files}. To easily understand the explanations in this section you can use @ref{The TEMPLATE program} which contains the bare minimum code for one program. This template can also be used to easily add new utilities. @menu * Mandatory source code files:: Description of files common to all programs. * The TEMPLATE program:: Template for easy creation of a new program. @end menu @node Mandatory source code files, The TEMPLATE program, Program source, Program source @subsection Mandatory source code files Some programs might need lots of source files and if there is no fixed convention, navigating them can become very hard for a new inquirer into the code. The following source files exist in every program's source directory (which is located in @file{bin/progname}). For small programs, these files are enough. Larger programs will need more files. In general for writing other source files, please choose filenames that are descriptive. @vtable @file @item main.c @cindex @code{main} function Each executable has a @code{main} function, which is located in @file{main.c}. Therefore this file in any program's source code will be the starting point. No actual processing functions are to be defined in this file, the function(s) in this file are only meant to connect the most high level steps of each program. Generally, @code{main} will first call the top user interface function to read user input and make all the preparations. Then it will pass control to the top processing function for that program. The functions to do both these jobs must be defined in other source files. @item main.h @cindex Top root structure @cindex @code{prognameparams} @cindex Root parameter structure @cindex Main parameters C structure All the major parameters which will be used in the program must be stored in a structure which is defined in @file{main.h}. The name of this structure is usually @code{prognameparams}, for example @code{imgcropparams}. So @code{#include "main.h"} will be a staple in all the source codes of the program and most of the functions. Keeping all the major parameters of a program in this structure has the major benefit that most functions will only need one argument: a pointer to this structure. This will significantly facilitate the job of the programmer, the inquirer and the computer. All the programs in Gnuastro are designed to be low-level, small and independent parts, so this structure should not get too large. The main root structure of a program contains at least two other structures: a structure only keeping parameters for user interface functions, which is also defined in @file{main.h} and the @code{commonparams} structure which is defined in @file{lib/gnuastro/commonparams.h}@footnote{ @file{lib/gnuastro/commonparams.h} is a program-specific header and not installed as part of the libraries.}. The main structure can become very large and since the programmer and inquirer often don't need to be confused with these parameters mixed with the actual processing parameters, they are conveniently defined in another structure which is named @code{uiparams} and is also defined in @file{main.h}. It could be defined in @file{ui.h} (see below) so the main functions remain completely ignorant to it, but its parameters might be needed for reporting input conditions, so it is included as part of the main program structure. @cindex @code{p} This top root structure is conveniently called @code{p} (short for parameters) by all the programs. The @code{uiparams} structure is called @code{up} (for user parameters) and the @code{commonparams} structure is called @code{cp}. With this convention any reader can immediately understand where to look for the definition of one parameter. @cindex Structure de-reference operator @cindex Operator, structure de-reference With this basic root structure, source code of functions can potentially become full of structure de-reference operators (@command{->}) which can make the code very un-readable. In order to avoid this, whenever a parameter is used more than a couple of times in a function, a parameter of the same type and with the same name (so it can be searched) as the desired parameter should be defined and put the value of the root structure inside of it in definition time. For example @example char *hdu=p->cp.hdu; int verb=p->cp.verb; @end example @item args.h @cindex Argp argument parser The argument parser structures (which are used by GNU C library's Argp) for each program are defined in @file{args.h}. They are separate global variables and function definitions that will be used by Argp. We recommend going through the appropriate section in GNU C library to understand their exact meaning, although they should be descriptive and understandable enough by looking at a few of the programs. @item ui.c, ui.h @cindex User interface functions @cindex Functions for user interface The user interface functions are also a unique set of functions in all the programs, so they are particularly named @file{ui.c} and @file{ui.h} in all the programs. Everything related to reading the user input arguments and options, checking the configuration files and checking the consistency of the input parameters before the actual program is run should be done in this file. Since most functions are the same, with only the internal checks and structure parameters differing, we recommend going through several of the examples and structuring your @file{ui.c} in a similar fashion with the rest of the programs. @cindex @code{setparams} function The most high-level function in @file{ui.c} is named @code{setparams} which accepts @code{int argc, char *argv[]} and a pointer to the root structure for that program, see the explanation for @file{main.h}. This is the function that @code{main} calls. The basic idea of the functions in this file is that the processing functions should need a minimum number of such checks. With this convention an inquirer who only wants to understand only one part (mostly the processing part and not user input details) of the code can easily do so. It also makes all the errors related to input appear before the processing begins which is more convenient for the user. @item progname.c @cindex Top processing source file The main processing functions in each program which keep the function(s) that @code{main()} will call are in a file named @file{progname.c}, for example @file{imgcrop.c} or @file{noisechisel.c}. The function within these files which @code{main()} calls is also named after the program, for example @example void imgcrop(struct imgcropparams *p) @end example @noindent or @example void noisechisel(struct noisechiselparams *p) @end example @noindent In this manner, if an inquirer is interested the processing steps, they can immediately come and check this file for the first processing step without having to go through @file{main.c} first. In most situations, any failure in any step of the programs will result in an informative error message and an immediate abort in the program. So there is no need for return values. Under more complicated situations where a return value might be necessary, @code{void} will be replaced with an @code{int} in the examples above. @item cite.h @cindex Citation information This file keeps the function to be called if the user runs any of the programs with @option{--cite}, see @ref{Operating modes}. @end vtable @node The TEMPLATE program, , Mandatory source code files, Program source @subsection The TEMPLATE program In the @code{Version controlled source}, the @file{bin/} directory contains the source code for each program in a separate sub-directory. The @file{bin/TEMPLATE} directory contains the bare-minimum files to create a new program. It can be used to understand the conventions described in @ref{Program source}, or to easily create a new program. The extra creativity offered by libraries comes at a cost: you have to actually write your @code{main} function in the programming language of your choice, and compile it before you can use it. You will also need to find a way to pass input and output information to the function. So when an operation has well-defined inputs and outputs and is commonly needed, it is much more worthwhile to simply do the work in a program (either by modifying an existing one or creating a new one), instead of the using underlying libraries every time. To define your new program based on this template, just take the following steps: @enumerate @item Select a name for your new program (for example @file{myprog}). @item Copy the @file{TEMPLATE} directory to a directory with your program's name: @example $ cp -R bin/TEMPLATE bin/myprog @end example @item Open @file{configure.ac} in the top Gnuastro source. This file manages the operations that are done when a user runs @file{./configure}. Going down the file, you will notice repetitive parts for each program. Copy one of those and correct the names of the copied program to your new program name. We follow alphabetic ordering here, so please place it correctly. There are multiple places where this has to be done, so be patient and go down to the bottom of the file. Ultimately add @file{bin/myprog/Makefile} to @code{AC_CONFIG_FILES}, only here the ordering depends on the length of the name. @item Open @file{Makefile.am} in the top Gnuastro source. Similar to the previous step, add your new program similar to all the other programs. @item Change @code{TEMPLATE} to @code{myprog} in the file names and contents of the files in the @file{bin/myprog/} directory. @item Run the following command to re-build the configuration and build system. @example $ autoreconf -f @end example Your new program will be built the next time you run @command{./configure} and @command{make}. @end enumerate @node Documentation, Building and debugging, Program source, Developing @section Documentation Documentation (this book) is an integral part of Gnuastro. Documentation is not considered a separate project. So, no change is considered valid for implementation unless the respective parts of the book have also been updated. The following procedure can be a good suggestion to take when you have a new idea and are about to start implementing it. The steps below are not a requirement, the important thing is that when you send the program to be included in Gnuastro, the book and the code have to both be fully up-to-date and compatible and the purpose should be very clearly explained. You can follow any path you choose to do this, the following path was what we found to be most successful during the initial design and implementation steps of Gnuastro. @enumerate @item Edit the book and fully explain your desired change, such that your idea is completely embedded in the general context of the book with no sense of discontinuity for a first time reader. This will allow you to plan the idea much more accurately and in the general context of Gnuastro or a particular program. Later on, when you are coding, this general context will significantly help you as a road-map. A very important part of this process is the program introduction, which explains the purposes of the program. Before actually starting to code, explain your idea's purpose thoroughly in the start of the program section you wish to add or edit. While actually writing its purpose for a new reader, you will probably get some very valuable ideas that you hadn't thought of before, this has occurred several times during the creation of Gnuastro. If an introduction already exists, embed or blend your idea's purpose with the existing purposes. We emphasize that doing this is equally useful for you (as the programmer) as it is useful for the user (reader). Recall that the purpose of a program is very important, see @ref{Program design philosophy}. As you have already noticed for every program, it is very important that the basics of the science and technique be explained in separate subsections prior to the `Invoking Programname' subsection. If you are writing a new program or your addition involves a new concept, also include such subsections and explain the concepts so a person completely unfamiliar with the concepts can get a general initial understanding. You don't have to go deep into the details, just enough to get an interested person (with absolutely no background) started. If you feel you can't do that, then you have probably not understood the concept yourself! Have in mind that your only limitation in length is the fatigue of the reader after reading a long text, nothing else. It might also help if you start implementing your idea in the `Invoking ProgramName' subsection (explaining the options and arguments you have in mind) at this stage too. Actually starting to write it here will really help you later when you are coding. @item After you have finished adding your initial intended plan to the book, then start coding your change or new program within the Gnuastro source files. While you are coding, you will notice that somethings should be different from what you wrote in the book (your initial plan). So correct them as you are actually coding. @item In the end, read the section in the book that you edited completely and see if you didn't miss any change in the coding and to see if the context is fairly continuous for a first time reader (who hasn't seen the book or had known of Gnuastro before you made your change). @end enumerate @node Building and debugging, Test scripts, Documentation, Developing @section Building and debugging @cindex GNU Libtool @cindex GNU Autoconf @cindex GNU Automake @cindex GNU build system To build the various programs and libraries in Gnuastro, the GNU build system is used which defines the steps in @ref{Quick start}. It consists of GNU Autoconf and GNU Automake and GNU Libtool which are collectively known as GNU Autotools. They provide a very portable system to check the environment a program is to be installed on prior to compiling and set the compilation conditions based on the particular user. They also make installing everything in their standard places very easy for the programmer. Most of the small caps files that you see in the top source directory of the tarball are created by these three tools (see @ref{Version controlled source}). @cindex @file{tmpfs-config-make} @cindex @file{tests/during-dev.sh} To facilitate the building and testing of your work during development, Gnuastro comes with two scripts: @file{tmpfs-config-make} and @file{tests/during-dev.sh}. The former is fully described in @ref{Configure and build in RAM}. During development, you would commonly run this command only once (at the start of your work). The latter is designed to be run each time you make a change and want to test your work (with some possible input and output). The script itself is heavily commented and thoroughly describes the best way to use it, so we won't repeat it here. As a summary: you specify the build directory, an output directory (for the built program to be run in and also contains the inputs), the program's short name and the arguments and options that it should be run with. This script will then build Gnuastro, go to the output directory and run the built executable from there. One option for the output directory might be your desktop, so you can easily see the output files and delete them when you are finished. The main purpose of these scripts is to keep your source directory clean and facilitate your development. @cindex Debugging @cindex Optimization By default all the programs are compiled with optimization flags for increased speed. A side effect of optimization is that valuable debugging information is lost. All the libraries are also linked as shared libraries by default. Shared libraries further complicate the debugging process and significantly slow down the compilation (the @command{make} command). So during development it is recommended to configure Gnuastro as follows: @example $ ./configure --disable-shared CFLAGS="-g -O0" @end example @noindent These options to configure are already included in @file{tmpfs-config-make}, you just have to un-comment them. In order to understand the building process, you can go through the Autoconf, Automake and Libtool manuals, like all GNU manuals they provide both a great tutorial and technical documentation. The ``A small Hello World'' section in Automake's manual (in chapter 2) can be a good starting guide after you have read the separate introductions. @node Test scripts, Developer's checklist, Building and debugging, Developing @section Test scripts @cindex Test scripts @cindex Gnuastro test scripts As explained in @ref{Tests}, for every program some simple tests are written to check the various independent features of the program. All the tests are placed in the @file{tests/} directory. There is one script (@file{prepconf.sh}) in this folder and several @file{Makefile}s. The script is the first `test' that will be run. It will copy all the configuration files from the various directories to a @file{.gnuastro} directory which it will make so the various tests can set the default values. For each program, the tests are placed inside directories with the program name. Each test is written as a shell script. The last line of this script is the test which runs the program with certain parameters. The return value of this script determines the fate of the test, see the ``Support for test suites'' chapter of the Automake manual for a very nice and complete explanation. In every script, two variables are defined at first: @code{prog} and @code{execname}. The first specifies the program name and the second the location of the executable. @cindex Build tree @cindex Source tree @cindex @file{tmpfs-config-make} The most important thing to have in mind about all the test scripts is that they are run from inside the @file{tests/} directory in the ``build tree''. Which can be different from the directory they are stored in (known as the ``source tree''). The @file{tmpfs-config-make} script uses this feature (see @ref{Configure and build in RAM}). This distinction is made by GNU Autoconf and Automake (which configure, build and install Gnuastro) so that you can install the program even if you don't have write access to the directory keeping the source files. See the ``Parallel build trees (a.k.a VPATH builds)'' in the Automake manual for a nice explanation. Because of this, any possible data that was not generated by other tests (and is thus in the build tree), for example the catalogs in ImageCrop tests, has a @command{$topsrc} prefix instead of @command{../} for the build three. This @command{$topsrc} variable points to the source tree where the script can find the source data (it is defined in @file{tests/Makefile.am}). The executables and other test products were built in the build tree (where they are being run), so they don't need to be prefixed with that variable. This is also true for images or files that were produced by other tests. @node Developer's checklist, Contributing to Gnuastro, Test scripts, Developing @section Developer's checklist This is a checklist of things to do after applying your changes/additions in Gnuastro: @enumerate @item If the change is non-trivial, write test(s) in the @file{tests/progname/} directory to test the change(s)/addition(s) you have made. Then add their file names to @file{tests/Makefile.am}. @item Run @command{$ make check} to make sure everything is working correctly. @item Make sure the documentation (this book) is completely up to date with your changes, see @ref{Documentation}. @item Commit your change to your issue branch (see @ref{Production workflow} and @ref{Forking tutorial}) Afterwards, run Autoreconf to generate the appropriate version number: @example $ autoreconf -f @end example @cindex Making a distribution package @item Finally, to make sure everything will be built, installed and checked correctly run @example $ make distcheck @end example @noindent This command will create a distribution file (ending with @file{.tar.gz}) and try to compile it in the most general cases, then it will run the tests on what it has built in its own mini-environment. If @command{$ make distcheck} finishes successfully, then you are safe to send your changes to us to implement or for your own purposes. See @ref{Production workflow} and @ref{Forking tutorial}. @end enumerate @node Contributing to Gnuastro, , Developer's checklist, Developing @section Contributing to Gnuastro You have this great idea or have found a good fix to a problem which you would like to implement in Gnuastro. You have also become familiar with the general design of Gnuastro in the previous sections of this chapter (see @ref{Developing}) and want to start working on and sharing your new addition/change with the whole community as part of the official release. This is great and your contribution is most welcome. This section and the next (see @ref{Developer's checklist}) are written in the hope of making it as easy as possible for you to share your great idea with the Gnuastro community. @cindex FSF @cindex Free Software Foundation In this section we discuss the final steps you have to take: legal and technical. From the legal perspective, the copyright of any work you do on Gnuastro has to be assigned to the Free Software Foundation (FSF) and the GNU operating system, or you have to sign a disclaimer. We do this to ensure that Gnuastro can remain free in the future, see @ref{Copyright assignment}. From the technical point of view, in this section we also discuss commit guidelines (@ref{Commit guidelines}) and the general version control workflow of Gnuastro in @ref{Production workflow}, along with a tutorial in @ref{Forking tutorial}. Recall that before starting the work on your idea, be sure to checkout the bugs and tasks trackers in @ref{Gnuastro project webpage} and announce your work there so you don't end up spending time on something others have already worked on, and also to attract similarly interested developers to help you. @menu * Copyright assignment:: Copyright has to be assigned to the FSF. * Commit guidelines:: Guidelines for commit messages. * Production workflow:: Submitting your commits (work) for inclusion. * Forking tutorial:: Tutorial on workflow steps with Git. @end menu @node Copyright assignment, Commit guidelines, Contributing to Gnuastro, Contributing to Gnuastro @subsection Copyright assignment Gnuastro's copyright is owned by the FSF. Professor Eben Moglen, of the Columbia University Law School has given a nice summary of the reasons for this at @url{https://www.gnu.org/licenses/why-assign}. Below we are copying it verbatim for self consistency (in case you are offline or reading in print). @quotation Under US copyright law, which is the law under which most free software programs have historically been first published, there are very substantial procedural advantages to registration of copyright. And despite the broad right of distribution conveyed by the GPL, enforcement of copyright is generally not possible for distributors: only the copyright holder or someone having assignment of the copyright can enforce the license. If there are multiple authors of a copyrighted work, successful enforcement depends on having the cooperation of all authors. In order to make sure that all of our copyrights can meet the record keeping and other requirements of registration, and in order to be able to enforce the GPL most effectively, FSF requires that each author of code incorporated in FSF projects provide a copyright assignment, and, where appropriate, a disclaimer of any work-for-hire ownership claims by the programmer's employer. That way we can be sure that all the code in FSF projects is free code, whose freedom we can most effectively protect, and therefore on which other developers can completely rely. @end quotation Please get in touch with the Gnuastro maintainer (currently Mohammad Akhlaghi, akhlaghi -at- gnu -dot- org) to follow the procedures. It is possible to do this for each change (good for for a single contribution), and also more generally for all the changes/additions you do in the future within Gnuastro. So if you have already assigned the copyright of your work on another GNU software to the FSF, it should be done again for Gnuastro. The FSF has staff working on these legal issues and the maintainer will get you in touch with them to do the paperwork. The maintainer will just be informed in the end so your contributions can be merged within the Gnuastro source code. Gnuastro will gratefully acknowledge (see @ref{Acknowledgments}) all the people who have assigned their copyright to the FSF and have thus helped to guarantee the freedom and reliability of Gnuastro. The Free Software Foundation will also acknowledge your copyright contributions in the Free Software Supporter: @url{https://www.fsf.org/free-software-supporter} which will circulate to a very large community (104,444 people in April 2016). See the archives for some examples and subscribe to receive interesting updates. The very active code contributors (or developers) will also be recognized as project members on the Gnuastro project webpage (see @ref{Gnuastro project webpage}) and can be given a @code{gnu.org} email address. So your very valuable contribution and copyright assignment will not be forgotten and is highly appreciated by a very large community. If you are reluctant to sign an assignment, a disclaimer is also acceptable. @cartouche @noindent @strong{Do I need a disclaimer from my university or employer?} It depends on the contract with your university or employer. From the FSF's @file{/gd/gnuorg/conditions.text}: ``If you are employed to do programming, or have made an agreement with your employer that says it owns programs you write, we need a signed piece of paper from your employer disclaiming rights to'' Gnuastro. The FSF's copyright clerk will kindly help you decide, please consult the following email address: ``assign -at- gnu -dot- org''. @end cartouche @node Commit guidelines, Production workflow, Copyright assignment, Contributing to Gnuastro @subsection Commit guidelines To be able to cleanly integrate your work with the other developers, @strong{never commit on the @file{master} branch} (see @ref{Production workflow} for a complete discussion and @ref{Forking tutorial} for a cookbook example). In short, leave @file{master} only for changes you fetch, or pull from the official repository (see @ref{Synchronizing}). In the Gnuastro commit messages, we strive to follow these standards. Note that in the early phases of Gnuastro's development, we are experimenting and so if you notice earlier commits don't satisfy some of the guidelines below, it is because they predate that guideline. @table @asis @item Commit title The commits have to start with one short descriptive title. The title is separated from the body with one blank line. Run @command{git log} to see some of the most recent commit messages as an example. In general, the title should satisfy the following conditions: @itemize @item It is best for the title to be short, about 60 (or even 50) characters. Most emulated command-line terminals are about 80 characters wide. However, we should also allow for the commit hashes which are printed in @command{git log --oneline}, and also branch names or the graph structure outputs of @command{git log} which are also commonly used. @item The title should not finish with any full-stops or periods (`@key{.}'). @end itemize @item Commit body @cindex Mailing list: gnuastro-commits The body of the commit message is separated from the title by one empty line. Recall that anyone who has subscribed to @command{gnuastro-commits} mailing list will get the commit in their email after it has been pushed to @file{master}. People will also read them when they synchronize with the main Gnuastro repository (see @ref{Synchronizing}). Finally, the commit messages will later be used to update the @file{NEWS} file on each release. Therefore the commit message body plays a very important role in the development of Gnuastro, so please adhere to the following guidelines. @itemize @item The body should be very descriptive. Start the commit message body by explaining what changes your commit makes from a user's perspective (added, changed, or removed options, or arguments to programs or libraries, or modified algorithms, or new installation step, or etc). @item @cindex Mailing list: gnuastro-commits Try to explain the committed contents as best as you can. Recall that the readers of your commit message do not necessarily have your current background. After some time you will also forget the context, so this request is not just for others@footnote{@url{http://catb.org/esr/writings/unix-koans/prodigy.html}}. Therefore be very descriptive and explain as much as possible: what the bug/task was, justify the way you fixed it and discuss other possible solutions that you might not have included. For the last item, it is best to discuss them thoroughly as comments in the appropriate section of the code, but only give a short summary in the commit message. Note that all added and removed source code lines will also be circulated in the @command{gnuastro-commits} mailing list. @item Like all other Gnuastro's text files, the lines in the commit body should not be longer than 75 characters, see @ref{Coding conventions}. This is to ensure that on standard terminal emulators (with 80 character width), the @command{git log} output can be cleanly displayed (note that the commit message is indented in the output of @command{git log}). If you use Emacs, Gnuastro's @file{.dir-locals.el} file will ensure that your commits satisfy this condition (using @key{M-q}). @item @cindex Mailing list: gnuastro-commits When the commit is related to a task or a bug, please include the respective ID (in the format of @code{bug/task #ID}, note the space) in the commit message (from @ref{Gnuastro project webpage}) for interested people to be able to followup the discussion that took place there. If the commit fixes a bug or finishes a task, the recommended way is to add a line after the body with `@code{This fixes bug #ID.}', or `@code{This finishes task #ID.}'. Don't assume that the reader has internet access to check the bug's full description when reading the commit message, so give a short introduction too. @end itemize @end table @node Production workflow, Forking tutorial, Commit guidelines, Contributing to Gnuastro @subsection Production workflow Fortunately `Pro Git' has done a wonderful job in explaining the different workflows in Chapter 5@footnote{@url{http://git-scm.com/book/en/v2/Distributed-Git-Distributed-Workflows}} and in particular the ``Integration-Manager Workflow'' explained there. The implementation of this workflow is nicely explained in Section 5.2@footnote{@url{http://git-scm.com/book/en/v2/Distributed-Git-Contributing-to-a-Project}} under ``Forked-Public-Project''. We have also prepared a short tutorial in @ref{Forking tutorial}. Anything on the master branch should always be tested and ready to be built and used. As described in `Pro Git', there are two methods for you to contribute to Gnuastro in the Integration-Manager Workflow: @enumerate @item You can send commit patches by email as fully explained in `Pro Git'. This is good for your first few contributions. Just note that raw patches (containing only the diff) do not have any meta-data (author name, date and etc). Therefore will not allow us to fully acknowledge your contributions as an author in Gnuastro: in the @file{AUTHORS} file and at the start of the PDF book. These author lists are created automatically from the version controlled source. To receive full acknowledgement when submitting a patch, is thus advised to use Git's @code{format-patch} tool. See Pro Git's @url{https://git-scm.com/book/en/v2/Distributed-Git-Contributing-to-a-Project#Public-Project-over-Email, Public project over email} section for a nice explanation. If you would like to get more heavily involved in Gnuastro's development, then you can try the next solution. @item You can have your own forked copy of Gnuastro on any hosting site you like (GitHub, GitLab, BitBucket, or etc) and inform us when your changes are ready so we merge them in Gnuastro. This is more suited for people who commonly contribute to the code (see @ref{Forking tutorial}). @end enumerate In both cases, your commits (with your name and information) will be preserved and your contributions will thus be fully recorded in the history of Gnuastro and in the @file{AUTHORS} file and this book (second page in the PDF format) once they have been incorporated into the official repository. Needless to say that in such cases, be sure to follow the bug or task trackers (or subscribe to the @command{gnuastro-devel} mailing list) and contact us before hand so you don't do something that someone else is already working on. In that case, you can get in touch with them and help the job go on faster, see @ref{Gnuastro project webpage}. This workflow is currently mostly borrowed from the general recommendations of Git@footnote{@url{https://github.com/git/git/blob/master/Documentation/SubmittingPatches}} and GitHub. But since Gnuastro is under heavy development currently, these might change and evolve to better suite our needs. @node Forking tutorial, , Production workflow, Contributing to Gnuastro @subsection Forking tutorial This is a tutorial on the second suggested method that you can submit your modifications in Gnuastro (see @ref{Production workflow}), which is commonly known as forking. Let's assume you want to start contributing to Gnuastro and you would like to use GitLab@footnote{See @url{https://www.gnu.org/software/repo-criteria-evaluation.html} for an evaluation of the major existing repositories.} to host your work remotely and share it with other Gnuastro developers once you are ready. You can create an empty repository on your hosting service webpage. If this is your first hosted repository on the webpage, you also have to upload your public SSH key@footnote{For example see this explanation provided by GitLab: @url{http://docs.gitlab.com/ce/ssh/README.html}.} for the @command{git push} command below to work. Here we'll assume you use the name @file{janedoe} to refer to yourself everywhere and that you choose @file{gnuastro-janedoe} as the name of your Gnuastro fork. Any online hosting service will give you an address (similar to `@file{git@@gitlab.com:}' below) of the empty repository you have created using their webpage, use that address in the third line below. @example $ git clone git://git.sv.gnu.org/gnuastro.git $ cd gnuastro $ git remote add janedoe git@@gitlab.com:janedoe/gnuastro-janedoe.git $ git push janedoe master @end example The full Gnuastro history is now pushed onto your hosting service and the @file{janedoe} remote is now also following your @file{master} branch. If you run @command{git remote show REMOTENAME} for the @file{origin} and @file{janedoe} remotes, you will see their difference: the first has pull access and the second doesn't. This nicely summarizes the main idea behind this workflow: you push to your remote repository, we pull from it and merge it into @file{master}, then you finalize it by pulling from the main repository. To test (compile) your changes during your work, you will need to bootstrap the version controlled source, see @ref{Bootstrapping} for a full description. The process above is only necessary for your first time setup, you don't need to repeat it. However, please repeat the steps below for each independent issue you intend to work on. Let's assume you have found a bug in @file{lib/statistics.c}'s median calculating function. You announce it (see @ref{Report a bug}) so everyone knows you are working on it. However, if it is a very simple, clear/obvious and straightforward bug to fix you can skip this initial announcement. With the commands below, you make a branch, checkout to it, correct the bug, check if it is indeed fixed, add it to the staging area, commit it to the new branch and push it to your hosting service. But before all of them, make sure that you are on the @file{master} branch and that your @file{master} branch is up to date with the main Gnuastro repository with the first two commands. @example $ git checkout master $ git pull $ git checkout -b bug-median-stats # Choose a descriptive name $ emacs lib/statistics.c $ # do your checks here $ git add lib/statistics.c $ git commit $ git push janedoe bug-median-stats @end example Your new branch is now on your hosted repository. Through the respective tacker on Savannah (see @ref{Gnuastro project webpage}) you can then let the other developers know that your @file{bug-median-stats} branch is ready. They will pull your work, test it themselves and if it is ready to be merged into the main Gnuastro history, they will merge it into the @file{master} branch. After that is done, you can simply checkout your local @file{master} branch and pull all the changes from the main repository. After the pull you can run `@command{git log}' as shown below, to see how @file{bug-median-stats} is merged with master. So you can push all the changes to your hosted repository and delete the branches: @example $ git checkout master $ git pull $ git log --oneline --graph --decorate --all $ git push janedoe master $ git branch -d bug-median-stats # delete local branch $ git push janedoe --delete bug-median-stats # delete remote branch @end example Just as a reminder, always keep your work on each issue in a separate local and remote branch so work can progress on them independently. After you make your announcement, other people might contribute to the branch before merging it in to @file{master}, so this is very important. Also before starting each issue branch from @file{master}, be sure to run @command{git pull} in @file{master} as shown above, to start your branch (work) from the most recent history point and thus simplify the final merging of your work. @node Gnuastro programs list, Other useful software, Developing, Top @appendix Gnuastro programs list GNU Astronomy Utilities @value{VERSION}, contains the following programs. They are sorted in alphabetical order and followed by their version number. A short description is provided for each program which starts with the executable names in @file{thisfont} followed by a link to the respective section in parenthesis, see @ref{Naming convention}. Throughout this book, they are ordered based on their context, please see the book contents for contextual ordering. @table @asis @item Arithmetic (@file{astarithmetic}, see @ref{Arithmetic}) For arithmetic operations on multiple (theoretically unlimited) number of datasets (images). It has a large and growing set of arithmetic, mathematical, and even statistical operators (for example @command{+}, @command{-}, @command{*}, @command{/}, @command{sqrt}, @command{log}, @command{min}, @command{average}, @command{median}). @item ConvertType (@file{astconvertt}, see @ref{ConvertType}) Convert astronomical data files (FITS or IMH) to and from several other standard image and data formats, for example TXT, JPEG, EPS or PDF. @item Convolve (@file{astconvolve}, see @ref{Convolve}) Convolve (blur or smooth) data with a given kernel in spatial and frequency domain on multiple threads. Convolve can also do de-convolution to find the appropriate kernel to PSF-match two images. @item CosmicCalculator (@file{astcosmiccal}, see @ref{CosmicCalculator}) Do cosmological calculations, for example the luminosity distance, distance modulus, comoving volume and many more. @item Header (@file{astheader}, see @ref{Header}) Print and manipulate the header data of a FITS file. @item ImageCrop (@file{astimgcrop}, see @ref{ImageCrop}) Crop region(s) from an image and stitch several images if necessary. Inputs can be in pixel coordinates or world coordinates. @item ImageStatistics (@file{astimgstat}, see @ref{ImageStatistics}) Get pixel statistics and save histogram and cumulative frequency plots. @item ImageWarp (@file{astimgwarp}, see @ref{ImageWarp}) Warp image to new pixel grid. Any projective transformation or Homography can be applied to the input images. @item MakeCatalog (@file{astmkcatalog}, see @ref{MakeCatalog}) Make catalog of labeled image (output of NoiseChisel). The catalogs are highly customizable and adding new calculations/columns is very straightforward. @item MakeNoise (@file{astmknoise}, see @ref{MakeNoise}) Make (add) noise to an image, with a large set of random number generators and any seed. @item MakeProfiles (@file{astmkprof}, see @ref{MakeProfiles}) Make mock 2D profiles in an image. The central regions of radial profiles are made with a configurable 2D Monte Carlo integration. It can also build the profiles on an over-sampled image. @item NoiseChisel (@file{astnoisechisel}, see @ref{NoiseChisel}) Detect and segment signal in noise. It uses a technique to detect very faint and diffuse, irregularly shaped signal in noise (galaxies in the sky), using thresholds that are below the Sky value, see @url{http://arxiv.org/abs/1505.01664, arXiv:1505.01664}. @item SubtractSky (@file{astsubtractsky}, @ref{SubtractSky}) Find and subtract sky value by comparing the mode and median on a mesh grid. @item Table (@file{asttable}, @ref{Table}) Convert FITS binary and ASCII tables into other such tables, print them on the command-line, save them in a plain text file, or get the FITS table information. @end table @node Other useful software, GNU Free Documentation License, Gnuastro programs list, Top @appendix Other useful software In this appendix the installation of programs and libraries that are not direct Gnuastro dependencies are discussed. However they can be useful for working with Gnuastro. @menu * SAO ds9:: Viewing FITS images. * PGPLOT:: Plotting directly in C @end menu @node SAO ds9, PGPLOT, Other useful software, Other useful software @section SAO ds9 @cindex SAO ds9 @cindex FITS image viewer SAO ds9@footnote{@url{http://ds9.si.edu/}} is not a requirement of Gnuastro, it is a FITS image viewer. So to check your inputs and outputs, it is one of the best options. Like the other packages, it might already be available in your distribution's repositories. It is already pre-compiled in the download section of its webpage. Once you download it you can unpack and install (move it to a system recognized directory) with the following commands (@code{x.x.x} is the version number): @example $ tar xf ds9.linux64.x.x.x.tar.gz $ sudo mv ds9 /usr/local/bin @end example Once you run it, there might be a complaint about the Xss library, which you can find in your distribution package management system. You might also get an @command{XPA} related error. In this case, you have to add the following line to your @file{~/.bashrc} and @file{~/.profile} file (you will have to log out and back in again for the latter): @example export XPA_METHOD=local @end example @menu * Viewing multiextension FITS:: Configure SAO ds9 for multiextension images. @end menu @node Viewing multiextension FITS, , SAO ds9, SAO ds9 @subsection Viewing multiextension FITS images @cindex Multiextention FITS @cindex Opening multiextention FITS The FITS definition allows for multiple extensions inside a FITS file, each extension can have a completely independent data set inside of it. If you ordinarily open a multi-extension FITS file with SAO ds9, for example by double clicking on the file or running @command{$ds9 foo.fits}, SAO ds9 will only show you the first extension. To be able to switch between the extensions you have to follow these menus in the SAO ds9 window: @clicksequence{File@click{}Open Other@click{}Open Multi Ext Cube} and then choose the Multi extension FITS file in your computer's file structure. @cindex @option{-mecube} (ds9) The method above is a little tedious to do every time you want view a multi-extension FITS file. Fortunately SAO ds9 also provides options that you can use to specify a particular behavior. One of those options is @option{-mecube} which opens a FITS image as a multi-extension data cube. So on the command-line, if you run @command{$ds9 -mecube foo.fits} a small window will also be opened, which allows you to switch between the image extensions that @file{foo.fits} might have. If @file{foo.fits} only consists of one extension, then SAO ds9 will open as usual. Just to avoid confusion, note that SAO ds9 does not follow the GNU style of separating long and short options as explained in @ref{Arguments and options}. In the GNU style, this `long' option should have been called like @option{--mecube}, but SAO ds9 does follow those conventions and has its own. @cindex GNOME 3 It is really convenient if you set ds9 to always run with the @option{-mecube} option on your graphical display. On GNOME 3 (the most popular graphic user interface for GNU/Linux systems) you can do this by taking the following steps: @itemize @item @cindex @file{.desktop} Open your favorite text editor and put the following text in a file that ends with @file{.desktop}, for example @file{saods9.desktop}. The file is very descriptive. @example [Desktop Entry] Type=Application Version=1.0 Name=SAO ds9 Comment=View FITS images Exec=ds9 -mecube %f Terminal=false Categories=Graphic;FITS; @end example @item Copy this file into your local (user) applications directory: @example $ cp saods9.desktop ~/.local/share/applications/ @end example In case you don't have the directory, you can make it yourself: @example $ mkdir -p ~/.local/share/applications/ @end example @item The steps above will add SAO ds9 as one of your applications. To make it default for every time you click on a FITS file. Right click on a FITS file and select ``Open With'', then go into ``Other Application...'' and choose ``SAO ds9''. @end itemize @cindex GNOME 2 In case you are using GNOME 2 you can take the following steps: right click on a FITS file and choose @clicksequence{Properties@click{}Open With@click{}Add} button. A list of applications will show up, ds9 might already be present in the list, but don't choose it because it will run with no options. Below the list is an option ``Use a custom command''. Click on it and write the following command: @command{ds9 -mecube} in the box and click ``Add''. Then finally choose the command you just added as the default and click the ``Close'' button. @node PGPLOT, , SAO ds9, Other useful software @section PGPLOT @cindex PGPLOT @cindex C, plotting @cindex Plotting directly in C PGPLOT is a package for making plots in C. It is not directly needed by Gnuastro, but can be used by WCSLIB, see @ref{WCSLIB}. As explained in @ref{WCSLIB}, you can install WCSLIB without it too. It is very old (the most recent version was released early 2001!), but remains one of the main packages for plotting directly in C. WCSLIB uses this package to make plots if you want it to make plots. If you are interested you can also use it for your own purposes. @cindex Python Matplotlib @cindex Matplotlib, Python @cindex PGFplots in @TeX{} or @LaTeX{} If you want your plotting codes in between your C program, PGPLOT is currently one of your best options. The recommended alternative to this method is to get the raw data for the plots in text files and input them into any of the various more modern and capable plotting tools separately, for example the Matplotlib library in Python or PGFplots in @LaTeX{}. This will also significantly help code readability. Let's get back to PGPLOT for the sake of WCSLIB. Installing it is a little tricky (mainly because it is so old!). You can download the most recent version from the FTP link in its webpage@footnote{@url{http://www.astro.caltech.edu/~tjp/pgplot/}}. You can unpack it with the @command{tar xf} command. Let's assume the directory you have unpacked it to is @file{PGPLOT}, most probably it is: @file{/home/username/Downloads/pgplot/}. open the @file{drivers.list} file: @example $ gedit drivers.list @end example @noindent Remove the @code{!} for the following lines and save the file in the end: @example PSDRIV 1 /PS PSDRIV 2 /VPS PSDRIV 3 /CPS PSDRIV 4 /VCPS XWDRIV 1 /XWINDOW XWDRIV 2 /XSERVE @end example @noindent Don't choose GIF or VGIF, there is a problem in their codes. Open the @file{PGPLOT/sys_linux/g77_gcc.conf} file: @example $ gedit PGPLOT/sys_linux/g77_gcc.conf @end example @noindent change the line saying: @code{FCOMPL="g77"} to @code{FCOMPL="gfortran"}, and save it. This is a very important step during the compilation of the code if you are in GNU/Linux. You now have to create a folder in @file{/usr/local}, don't forget to replace @file{PGPLOT} with your unpacked address: @example $ su # mkdir /usr/local/pgplot # cd /usr/local/pgplot # cp PGPLOT/drivers.list ./ @end example To make the Makefile, type the following command: @example # PGPLOT/makemake PGPLOT linux g77_gcc @end example @noindent It should finish by saying: @command{Determining object file dependencies}. You have done the hard part! The rest is easy: run these three commands in order: @example # make # make clean # make cpg @end example Finally you have to place the position of this directory you just made into the @command{LD_LIBRARY_PATH} environment variable and define the environment variable @command{PGPLOT_DIR}. To do that, you have to edit your @file{.bashrc} file: @example $ cd ~ $ gedit .bashrc @end example @noindent Copy these lines into the text editor and save it: @cindex @file{LD_LIBRARY_PATH} @example PGPLOT_DIR="/usr/local/pgplot/"; export PGPLOT_DIR LD_LIBRARY_PATH=$LD_LIBRARY_PATH:/usr/local/pgplot/ export LD_LIBRARY_PATH @end example @noindent You need to log out and log back in again so these definitions take effect. After you logged back in, you want to see the result of all this labor, right? Tim Pearson has done that for you, create a temporary folder in your home directory and copy all the demonstration files in it: @example $ cd ~ $ mkdir temp $ cd temp $ cp /usr/local/pgplot/pgdemo* ./ $ ls @end example You will see a lot of pgdemoXX files, where XX is a number. In order to execute them type the following command and drink your coffee while looking at all the beautiful plots! You are now ready to create your own. @example $ ./pgdemoXX @end example @node GNU Free Documentation License, Index, Other useful software, Top @appendix GNU Free Documentation License @cindex GNU Free Documentation License @include fdl.texi @c Print the index and finish: @node Index, , GNU Free Documentation License, Top @unnumbered Index: Macros, structures and functions All Gnuastro library's exported macros start with @code{GAL_}, and its exported structures and functions start with @code{gal_}. This abbreviation stands for @emph{G}NU @emph{A}stronomy @emph{L}ibrary. The next element in the name is the name of the header which declares or defines them, so to use the @code{gal_array_fset_const} function, you have to @code{#include }. See @ref{Gnuastro library} for more. The @code{pthread_barrier} constructs are our implementation and are only available on systems that don't have them, see @ref{Implementation of pthread_barrier}. @printindex fn @unnumbered Index @printindex cp @bye gnuastro-0.2.33-8a3b/doc/README0000644000175000017500000000371412722534072012553 00000000000000Documentation of GNU Astronomy Utilities ======================================== This directory contains the documentation (manual) of GNU Astronomy Utilities (Gnuastro) and also all the files necessary for the Gnuastro webpage. Note that only the basic files needed to make the webpage are version controlled. The generated files are not. Documentation (manual): ----------------------- The documentation of Gnuastro is written in Texinfo. The main source file is `gnuastro.texi'. Webpage (only for maintainer) ----------------------------- The top Gnuastro webpage files are also held here, after all, a webpage is another form of documentation. To update the webpage, run the following script: $ ./forwebpage This script will generate the webpage using Gnulib's gendocs.sh script (which was part of the bootstrapping process), then it will copy them all in a specified directory anywhere you like (specified by the TOPWEBCHECKOUT shell variable). You don't have to version control any of the files in that directory, but it is easiest to have a fixed place since CVS needs a local copy. Unfortunately the GNU webpage runs on CVS! Read the top comments of the `forwebpage' script for instructions on what to do for the first time and later times. Update MathJax (for the webpage, only for maintainer) ----------------------------------------------------- There is a script in the `MathJax' directory on the Gnuastro webpage directory to update MathJax (`addmissing.sh'). You can get a recent version of MathJax from its webpage and put it in the correct place (see the comments in the script). 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GNULIB_FMOD = @GNULIB_FMOD@ GNULIB_FMODF = @GNULIB_FMODF@ GNULIB_FMODL = @GNULIB_FMODL@ GNULIB_FOPEN = @GNULIB_FOPEN@ GNULIB_FPRINTF = @GNULIB_FPRINTF@ GNULIB_FPRINTF_POSIX = @GNULIB_FPRINTF_POSIX@ GNULIB_FPURGE = @GNULIB_FPURGE@ GNULIB_FPUTC = @GNULIB_FPUTC@ GNULIB_FPUTS = @GNULIB_FPUTS@ GNULIB_FREAD = @GNULIB_FREAD@ GNULIB_FREOPEN = @GNULIB_FREOPEN@ GNULIB_FREXP = @GNULIB_FREXP@ GNULIB_FREXPF = @GNULIB_FREXPF@ GNULIB_FREXPL = @GNULIB_FREXPL@ GNULIB_FSCANF = @GNULIB_FSCANF@ GNULIB_FSEEK = @GNULIB_FSEEK@ GNULIB_FSEEKO = @GNULIB_FSEEKO@ GNULIB_FSTAT = @GNULIB_FSTAT@ GNULIB_FSTATAT = @GNULIB_FSTATAT@ GNULIB_FSYNC = @GNULIB_FSYNC@ GNULIB_FTELL = @GNULIB_FTELL@ GNULIB_FTELLO = @GNULIB_FTELLO@ GNULIB_FTRUNCATE = @GNULIB_FTRUNCATE@ GNULIB_FUTIMENS = @GNULIB_FUTIMENS@ GNULIB_FWRITE = @GNULIB_FWRITE@ GNULIB_GETC = @GNULIB_GETC@ GNULIB_GETCHAR = @GNULIB_GETCHAR@ GNULIB_GETCWD = @GNULIB_GETCWD@ GNULIB_GETDELIM = @GNULIB_GETDELIM@ GNULIB_GETDOMAINNAME = @GNULIB_GETDOMAINNAME@ GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = 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$(toputildir)/imgstat/astimgstat man/astimgwarp.1: $(top_srcdir)/bin/imgwarp/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "warp (transform) input image" \ --libtool $(toputildir)/imgwarp/astimgwarp man/astmkcatalog.1: $(top_srcdir)/bin/mkcatalog/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "Make a catalog from labeled input images" \ --libtool $(toputildir)/mkcatalog/astmkcatalog man/astmknoise.1: $(top_srcdir)/bin/mknoise/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "add noise to an image" \ --libtool $(toputildir)/mknoise/astmknoise man/astmkprof.1: $(top_srcdir)/bin/mkprof/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "make standard 2D profiles on an image" \ --libtool $(toputildir)/mkprof/astmkprof man/astnoisechisel.1: $(top_srcdir)/bin/noisechisel/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "detect signal in a noisy image" \ --libtool $(toputildir)/noisechisel/astnoisechisel man/astsubtractsky.1: $(top_srcdir)/bin/subtractsky/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "subtract the sky value in 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The problem is that when you use braces in the TeX commands, Texinfo will complain for other formats and when you quote the braces with the at sign, e.g. @{, then TeX will not see the brace properly. So I made two macro functions: mymath{} and dispmath{}. The first is for inline math and the second is for display math where the equation has a line of its own. For the other formats, everything is normal, except the display math equations that don't have any proper solution, so I have just put a $$ $$ around the math. Copying and distribution of this file, with or without modification, are permitted in any medium without royalty provided the copyright notice and this notice are preserved. This file is offered as-is, without any warranty. @end ignore @c HTML: @ifhtml @macro mymath{arg} @inlineraw{html,\\(\arg\\\)} @end macro @macro dispmath{arg} @inlineraw{html,$$\arg\$$} @end macro @end ifhtml @c Docbook @ifdocbook @macro mymath{arg} @math{\arg\} @end macro @macro dispmath{arg} @center@inlineraw{docbook,$$\arg\$$} @end macro @end ifdocbook @c info and plaintext @ifinfo @macro mymath{arg} @inlineraw{info,$\arg\$} @end macro @macro dispmath{arg} @center@inlineraw{info,$$\arg\$$} @end macro @end ifinfo @c TeX @iftex @macro mymath{arg} @math{\arg\} @end macro @macro dispmath{arg} @tex $$\arg\$$ @end tex @end macro @end iftex gnuastro-0.2.33-8a3b/doc/stamp-vti0000644000175000017500000000015713004464676013546 00000000000000@set UPDATED 25 October 2016 @set UPDATED-MONTH October 2016 @set EDITION 0.2.33-8a3b @set VERSION 0.2.33-8a3b gnuastro-0.2.33-8a3b/doc/version.texi0000644000175000017500000000015713004442335014243 00000000000000@set UPDATED 25 October 2016 @set UPDATED-MONTH October 2016 @set EDITION 0.2.33-8a3b @set VERSION 0.2.33-8a3b gnuastro-0.2.33-8a3b/doc/Makefile.am0000644000175000017500000001502513003421401013705 00000000000000## Process this file with automake to produce Makefile.inx ## ## This is part of GNU Astronomy Utilities (gnuastro). It will be ## called by the Makefile.am in the top directory. ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## GNU Astronomy Utilities is free software: you can redistribute it ## and/or modify it under the terms of the GNU General Public License ## as published by the Free Software Foundation, either version 3 of ## the License, or (at your option) any later version. ## ## GNU Astronomy Utilities is distributed in the hope that it will be ## useful, but WITHOUT ANY WARRANTY; without even the implied warranty ## of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the ## GNU General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with GNU Astronomy Utilities. If not, see ## . ## Set the shell SHELL=/bin/bash BUILT_SOURCES = $(srcdir)/authors.texi ## fdl.texi (The GNU Free documentation license in Texinfo format) is ## bootstrapped from Gnulib. Therefore it is not in this ## directory. However, it is needed by gnuastro.texi to build the ## documentation. It is the job of AM_MAKEINFOFLAGS, to pass options to the ## documentation build programs. BOOTSTRPDOC is defined in `configure.ac'. bootstrpdoc = $(top_srcdir)/bootstrapped/doc AM_MAKEINFOFLAGS = -I $(bootstrpdoc) -I $(srcdir) # This is just a temporary work-around since Automake does not pass the # AM_MAKEINFOFLAGS to texi2dvi (which builds DVI and PDF outputs). This was # reported in Automake's bug 23599. Note that a space is necessary between # the `-I' and directory for texi2dvi. TEXI2DVI = texi2dvi -I $(bootstrpdoc) -I $(srcdir) ## Commands to make the texinfo tools. info_TEXINFOS = gnuastro.texi gnuastro_TEXINFOS = $(bootstrpdoc)/fdl.texi formath.texi \ $(srcdir)/authors.texi ## Files not predefined by Automake, and not in dependencies that must ## be included in the final tar-ball distribution. EXTRA_DIST = genauthors README ## We want to build the authors.texi file only when we are building in the ## version controlled source. For the non version controlled souce, ## deleting this file is like somehow deleting formath.texi, it will not be ## rebuilt and result in an error. $(srcdir)/authors.texi: $(top_srcdir)/configure $(top_srcdir)/doc/genauthors $(top_srcdir) ## Images: infognuastrodir=$(infodir)/gnuastro-figures/ dist_infognuastro_DATA = $(top_srcdir)/doc/gnuastro-figures/* ## Man pages: to keep things managable, sort the utilities alphabetically. dist_man_MANS = man/astarithmetic.1 man/astconvertt.1 man/astconvolve.1 \ man/astcosmiccal.1 man/astheader.1 man/astimgcrop.1 man/astimgstat.1 \ man/astimgwarp.1 man/astmkcatalog.1 man/astmknoise.1 man/astmkprof.1 \ man/astnoisechisel.1 man/astsubtractsky.1 man/asttable.1 ## See if help2man is present or not. When help2man doesn't exist, we don't ## want to overwhelm the user with any commands, so we just let them know ## that the distributed man pages will be used. if COND_HASHELP2MAN MAYBE_HELP2MAN = help2man --output=$@ --source="$(PACKAGE_STRING)" else MAYBE_HELP2MAN = @echo "Using distributed man page for" endif # Build the `man' directory and then put all the man pages in # it. Unfortunately as far as I know, pattern rules are not portable in all # implementations of Make, so we have to list all the utilities manually. toputildir=$(top_builddir)/bin ALLMANSDEP = $(top_srcdir)/lib/commonargs.h man/astarithmetic.1: $(top_srcdir)/bin/arithmetic/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "arithmetic operations on images and numbers" \ --libtool $(toputildir)/arithmetic/astarithmetic man/astconvertt.1: $(top_srcdir)/bin/convertt/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "convert known data types to each other" \ --libtool $(toputildir)/convertt/astconvertt man/astconvolve.1: $(top_srcdir)/bin/convolve/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "convolve an image with a given kernel" \ --libtool $(toputildir)/convolve/astconvolve man/astcosmiccal.1: $(top_srcdir)/bin/cosmiccal/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "estimate cosmological values" \ --libtool $(toputildir)/cosmiccal/astcosmiccal man/astheader.1: $(top_srcdir)/bin/header/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "view and manipulate FITS headers" \ --libtool $(toputildir)/header/astheader man/astimgcrop.1: $(top_srcdir)/bin/imgcrop/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "crop regions of an image" \ --libtool $(toputildir)/imgcrop/astimgcrop man/astimgstat.1: $(top_srcdir)/bin/imgstat/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "get image statistics" \ --libtool $(toputildir)/imgstat/astimgstat man/astimgwarp.1: $(top_srcdir)/bin/imgwarp/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "warp (transform) input image" \ --libtool $(toputildir)/imgwarp/astimgwarp man/astmkcatalog.1: $(top_srcdir)/bin/mkcatalog/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "Make a catalog from labeled input images" \ --libtool $(toputildir)/mkcatalog/astmkcatalog man/astmknoise.1: $(top_srcdir)/bin/mknoise/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "add noise to an image" \ --libtool $(toputildir)/mknoise/astmknoise man/astmkprof.1: $(top_srcdir)/bin/mkprof/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "make standard 2D profiles on an image" \ --libtool $(toputildir)/mkprof/astmkprof man/astnoisechisel.1: $(top_srcdir)/bin/noisechisel/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "detect signal in a noisy image" \ --libtool $(toputildir)/noisechisel/astnoisechisel man/astsubtractsky.1: $(top_srcdir)/bin/subtractsky/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "subtract the sky value in an image" \ --libtool $(toputildir)/subtractsky/astsubtractsky man/asttable.1: $(top_srcdir)/bin/table/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "read and write ASCII and FITS tables" \ --libtool $(toputildir)/table/asttable #man/astTEMPLATE.1: $(top_srcdir)/bin/TABLE/args.h $(ALLMANSDEP) # $(MAYBE_HELP2MAN) -n "put a short description here" \ $(toputildir)/TEMPLATE/astTEMPLATE gnuastro-0.2.33-8a3b/doc/man/0000755000175000017500000000000013004464725012522 500000000000000gnuastro-0.2.33-8a3b/doc/man/asttable.10000644000175000017500000000776413004464676014346 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.3. .TH TABLE "1" "October 2016" "GNU Astronomy Utilities 0.2.33-8a3b" "User Commands" .SH NAME Table \- read and write ASCII and FITS tables .SH SYNOPSIS .B asttable [\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR .SH DESCRIPTION Table is part of GNU Astronomy Utilities 0.2.33\-8a3b. Table prints (in a human readable format) a FITS table or its information. The output columns can either be selected by number, name or using regular expressions. The format of their printing can also be set (based on the type of data in the column). .PP For more information, please run any of the following commands. They will respectively show you the `Invoking Table' subsection, the complete `Table' section, or the full GNU Astronomy Utilities manual. In particular the first contains a very complete explanation of each option. .IP info asttable .IP info Table .IP info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP info help\-gnuastro .PP Table options: .IP Input: .TP \fB\-c\fR, \fB\-\-column\fR=\fI\,STR\/\fR Input column name, number or regular expression. .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR Extension name or number of input data. .TP \fB\-I\fR, \fB\-\-ignorecase\fR Ignore case when matching column names. .IP Output: .TP \fB\-\-doubleprecision\fR=\fI\,INT\/\fR `double' column(s) precision. .TP \fB\-\-doublewidth\fR=\fI\,INT\/\fR `double' column(s) width (num charachers). .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-\-feg\fR=\fI\,STR\/\fR `f': only decimals, `e': scientific, `g': either. .TP \fB\-\-floatprecision\fR=\fI\,INT\/\fR `float' column(s) precision. .TP \fB\-\-floatwidth\fR=\fI\,INT\/\fR `float' column(s) width (num charachers). .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Do not remove input's dir info for output. .TP \fB\-\-lintwidth\fR=\fI\,INT\/\fR Longer integer column(s) width (num charachers). .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output file or directory name. .TP \fB\-\-sintwidth\fR=\fI\,INT\/\fR Shorter integer column(s) width (num charachers). .TP \fB\-\-strwidth\fR=\fI\,INT\/\fR String column(s) width (num charachers). .TP \fB\-t\fR, \fB\-\-fitstabletype\fR=\fI\,STR\/\fR Only `ascii', or `binary' are acceptable. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for Table. .TP \fB\-i\fR, \fB\-\-information\fR Only print table and columns information. .TP \fB\-\-nolog\fR No log file for programs which make one. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlydirconf\fR Only read current directory configuration file. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is this. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH AUTHOR Written by Mohammad Akhlaghi .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2016, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .SH "SEE ALSO" The full documentation for .B Table is maintained as a Texinfo manual. If the .B info and .B Table programs are properly installed at your site, the command .IP .B info Table .PP should give you access to the complete manual. gnuastro-0.2.33-8a3b/doc/man/astsubtractsky.10000644000175000017500000001146313004464676015624 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.3. .TH SUBTRACTSKY "1" "October 2016" "GNU Astronomy Utilities 0.2.33-8a3b" "User Commands" .SH NAME SubtractSky \- subtract the sky value in an image .SH SYNOPSIS .B astsubtractsky [\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR .SH DESCRIPTION SubtractSky is part of GNU Astronomy Utilities 0.2.33\-8a3b. SubtractSky Finds the sky value over a grid on the input and subtracts it from the image to give a clear and uniform output. .PP For more information, please run any of the following commands. They will respectively show you the `Invoking SubtractSky' subsection, the complete `SubtractSky' section, or the full GNU Astronomy Utilities manual. In particular the first contains a very complete explanation of each option. .IP info astsubtractsky .IP info SubtractSky .IP info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP info help\-gnuastro .PP SubtractSky options: .IP Input: .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR Extension name or number of input data. .TP \fB\-H\fR, \fB\-\-mhdu\fR=\fI\,STR\/\fR Mask image header name. .TP \fB\-k\fR, \fB\-\-kernel\fR=\fI\,STR\/\fR Kernel image file name for convolution. .TP \fB\-M\fR, \fB\-\-mask\fR=\fI\,STR\/\fR Mask image file name. .TP \fB\-U\fR, \fB\-\-khdu\fR=\fI\,STR\/\fR Kernel image header name for convolution. .IP Output: .TP \fB\-\-checkconvolution\fR Store convolved image in `_conv.fits' file. .TP \fB\-\-checksky\fR Store final sky and its STD in `_sky.fits' file. .TP \fB\-\-checkskystd\fR Include sky standard deviation in all checks too. .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Do not remove input's dir info for output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output file or directory name. .IP Mesh grid: .TP \fB\-a\fR, \fB\-\-nch1\fR=\fI\,INT\/\fR Number of channels along first FITS axis. .TP \fB\-b\fR, \fB\-\-nch2\fR=\fI\,INT\/\fR Number of channels along second FITS axis. .TP \fB\-\-checkmesh\fR Store mesh IDs in `_mesh.fits' file. .TP \fB\-d\fR, \fB\-\-mirrordist\fR=\fI\,FLT\/\fR Distance beyond mirror point. Multiple of std. .TP \fB\-\-fullconvolution\fR Ignore channels in imageconvolution. .TP \fB\-\-fullinterpolation\fR Ignore channels in interpolation. .TP \fB\-\-fullsmooth\fR Ignore channels in smoothing. .TP \fB\-\-interponlyblank\fR Only interpolate over the blank pixels. .TP \fB\-L\fR, \fB\-\-lastmeshfrac\fR=\fI\,INT\/\fR Fraction of last mesh area to add new. .TP \fB\-\-meshbasedcheck\fR Each mesh in one pixel in mesh check images. .TP \fB\-n\fR, \fB\-\-numnearest\fR=\fI\,INT\/\fR Number of nearest neighbors to interpolate. .TP \fB\-Q\fR, \fB\-\-minmodeq\fR=\fI\,FLT\/\fR Minimum acceptable quantile for the mode. .TP \fB\-s\fR, \fB\-\-meshsize\fR=\fI\,INT\/\fR Size of each mesh (tile) in the grid. .TP \fB\-T\fR, \fB\-\-smoothwidth\fR=\fI\,INT\/\fR Width of smoothing kernel (odd number). .IP Statistics: .HP \fB\-t\fR, \fB\-\-sigcliptolerance\fR=\fI\,FLT\/\fR Difference in STD tolerance to halt iteration. .TP \fB\-u\fR, \fB\-\-sigclipmultip\fR=\fI\,FLT\/\fR Multiple of standard deviation in sigma\-clipping. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for SubtractSky. .TP \fB\-\-nolog\fR No log file for programs which make one. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlydirconf\fR Only read current directory configuration file. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is this. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH AUTHOR Written by Mohammad Akhlaghi .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2016, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .SH "SEE ALSO" The full documentation for .B SubtractSky is maintained as a Texinfo manual. If the .B info and .B SubtractSky programs are properly installed at your site, the command .IP .B info SubtractSky .PP should give you access to the complete manual. gnuastro-0.2.33-8a3b/doc/man/astnoisechisel.10000644000175000017500000001616513004464676015557 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.3. .TH NOISECHISEL "1" "October 2016" "GNU Astronomy Utilities 0.2.33-8a3b" "User Commands" .SH NAME NoiseChisel \- detect signal in a noisy image .SH SYNOPSIS .B astnoisechisel [\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR .SH DESCRIPTION NoiseChisel is part of GNU Astronomy Utilities 0.2.33\-8a3b. NoiseChisel Detects and segments signal that is deeply burried in noise. It employs a noise\-based detection and segmentation method enabling it to be very resilient to the rich diversity of shapes in astronomical targets. .PP For more information, please run any of the following commands. They will respectively show you the `Invoking NoiseChisel' subsection, the complete `NoiseChisel' section, or the full GNU Astronomy Utilities manual. In particular the first contains a very complete explanation of each option. .IP info astnoisechisel .IP info NoiseChisel .IP info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP info help\-gnuastro .PP NoiseChisel options: .IP Input: .TP \fB\-B\fR, \fB\-\-minbfrac\fR=\fI\,FLT\/\fR Minimum fraction of undetected area in a mesh. .TP \fB\-E\fR, \fB\-\-skysubtracted\fR Input is already sky subtracted. .TP \fB\-F\fR, \fB\-\-minnumfalse\fR=\fI\,INT\/\fR Min No. of false detection/segments for quantile. .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR Extension name or number of input data. .TP \fB\-H\fR, \fB\-\-mhdu\fR=\fI\,STR\/\fR Mask image header name. .TP \fB\-k\fR, \fB\-\-kernel\fR=\fI\,STR\/\fR Kernel image file name. .TP \fB\-M\fR, \fB\-\-mask\fR=\fI\,STR\/\fR Mask image file name. .TP \fB\-U\fR, \fB\-\-khdu\fR=\fI\,STR\/\fR Kernel image header name. .IP Output: .TP \fB\-C\fR, \fB\-\-grownclumps\fR Save grownclumps instead of original clumps. .TP \fB\-\-detectonly\fR Do not do any segmentation. .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Do not remove input's dir info for output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output file or directory name. .IP Mesh grid: .TP \fB\-a\fR, \fB\-\-nch1\fR=\fI\,INT\/\fR Number of channels along first FITS axis. .TP \fB\-b\fR, \fB\-\-nch2\fR=\fI\,INT\/\fR Number of channels along second FITS axis. .TP \fB\-\-checkmesh\fR Store mesh IDs in `_mesh.fits' file. .TP \fB\-d\fR, \fB\-\-mirrordist\fR=\fI\,FLT\/\fR Distance beyond mirror point. Multiple of std. .TP \fB\-\-fullconvolution\fR Ignore channels in convolution. .TP \fB\-\-fullinterpolation\fR Ignore channels in interpolation. .TP \fB\-\-fullsmooth\fR Ignore channels in smoothing. .TP \fB\-\-interponlyblank\fR Only interpolate over the blank pixels. .TP \fB\-l\fR, \fB\-\-lmeshsize\fR=\fI\,INT\/\fR Size of each large mesh (tile) in the grid. .TP \fB\-L\fR, \fB\-\-lastmeshfrac\fR=\fI\,INT\/\fR Fraction of last mesh area to add new. .TP \fB\-\-meshbasedcheck\fR Each mesh in one pixel in mesh check images. .TP \fB\-n\fR, \fB\-\-numnearest\fR=\fI\,INT\/\fR Number of nearest neighbors to interpolate. .TP \fB\-Q\fR, \fB\-\-minmodeq\fR=\fI\,FLT\/\fR Minimum acceptable quantile for the mode. .TP \fB\-s\fR, \fB\-\-smeshsize\fR=\fI\,INT\/\fR Size of each small mesh (tile) in the grid. .TP \fB\-T\fR, \fB\-\-smoothwidth\fR=\fI\,INT\/\fR Width of smoothing kernel (odd number). .IP Detection: .TP \fB\-c\fR, \fB\-\-detquant\fR=\fI\,FLT\/\fR False detections S/N quantile to find the true. .TP \fB\-\-checkdetection\fR False detection steps in file `_det.fits'. .TP \fB\-\-checkdetectionsky\fR Sky for false detections in file `_detsky.fits'. .TP \fB\-\-checkmaskdet\fR Mask detections and sky, `_maskdet.fits'. .TP \fB\-\-checksky\fR Final sky and its STD per pixel `_sky.fits'. .TP \fB\-\-checkthreshold\fR Threshold value on each mesh `_thresh.fits'. .TP \fB\-\-detsnhistnbins\fR=\fI\,INT\/\fR Det. S/N histogram bins, suffix `_detsn.txt'. .TP \fB\-e\fR, \fB\-\-erode\fR=\fI\,INT\/\fR Num. erosions to apply after thresholding. .TP \fB\-\-erodengb\fR=\fI\,4or8\/\fR Use 4 or 8 connectivity in erosion. .TP \fB\-i\fR, \fB\-\-detsnminarea\fR=\fI\,INT\/\fR Minimum area to calculate S/N in detection. .TP \fB\-I\fR, \fB\-\-dilate\fR=\fI\,INT\/\fR Number of times to dilate true detections. .TP \fB\-\-noerodequant\fR=\fI\,FLT\/\fR Quantile for no erosion. .TP \fB\-\-openingngb\fR=\fI\,4or8\/\fR Use 4 or 8 connectivity in opening. .TP \fB\-p\fR, \fB\-\-opening\fR=\fI\,INT\/\fR Depth of opening to apply after erosion. .HP \fB\-r\fR, \fB\-\-sigcliptolerance\fR=\fI\,FLT\/\fR Difference in STD tolerance to halt iteration. .TP \fB\-R\fR, \fB\-\-dthresh\fR=\fI\,FLT\/\fR Threshold (STD multiple) for false detections. .TP \fB\-t\fR, \fB\-\-qthresh\fR=\fI\,FLT\/\fR Quantile threshold on convolved image. .TP \fB\-u\fR, \fB\-\-sigclipmultip\fR=\fI\,FLT\/\fR Multiple of standard deviation in sigma\-clipping. .IP Segmentation: .TP \fB\-\-checksegmentation\fR Store segmentation steps in file `_seg.fits'. .HP \fB\-\-clumpsnhistnbins\fR=\fI\,INT\/\fR Clump S/N histogram bins, suffix `_clumpsn.txt'. .TP \fB\-g\fR, \fB\-\-segquant\fR=\fI\,FLT\/\fR Signal to noise ratio quantile for clumps. .TP \fB\-G\fR, \fB\-\-gthresh\fR=\fI\,FLT\/\fR Threshold (STD multiple) to stop growing clumps. .TP \fB\-m\fR, \fB\-\-segsnminarea\fR=\fI\,INT\/\fR Minimum area to find clumps S/N. .TP \fB\-O\fR, \fB\-\-objbordersn\fR=\fI\,FLT\/\fR Minimum S/N for grown clumps to be one object. .TP \fB\-v\fR, \fB\-\-keepmaxnearriver\fR Keep clumps with max touching river. .TP \fB\-y\fR, \fB\-\-minriverlength\fR Minimum length of useful rivers in grown clumps. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for NoiseChisel. .TP \fB\-\-nolog\fR No log file for programs which make one. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlydirconf\fR Only read current directory configuration file. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is this. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH AUTHOR Written by Mohammad Akhlaghi .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2016, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .SH "SEE ALSO" The full documentation for .B NoiseChisel is maintained as a Texinfo manual. If the .B info and .B NoiseChisel programs are properly installed at your site, the command .IP .B info NoiseChisel .PP should give you access to the complete manual. gnuastro-0.2.33-8a3b/doc/man/astmkprof.10000644000175000017500000001376013004464676014546 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.3. .TH MAKEPROFILES "1" "October 2016" "GNU Astronomy Utilities 0.2.33-8a3b" "User Commands" .SH NAME MakeProfiles \- make standard 2D profiles on an image .SH SYNOPSIS .B astmkprof [\fI\,OPTION\/\fR...] [\fI\,BackgroundImage\/\fR] \fI\,Catalog\/\fR .SH DESCRIPTION MakeProfiles is part of GNU Astronomy Utilities 0.2.33\-8a3b. MakeProfiles will create a FITS image containing any number of mock astronomical profiles based on an input catalog. All the profiles will be built from the center outwards. First by Monte Carlo integration, then using the central pixel position. The tolerance level specifies when to switch to a latter. .PP For more information, please run any of the following commands. They will respectively show you the `Invoking MakeProfiles' subsection, the complete `MakeProfiles' section, or the full GNU Astronomy Utilities manual. In particular the first contains a very complete explanation of each option. .IP info astmkprof .IP info MakeProfiles .IP info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP info help\-gnuastro .PP MakeProfiles options: .IP Input: .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR Extension name or number of input data. .IP Output: .TP \fB\-C\fR, \fB\-\-inputascanvas\fR Use input image for output size and WCS. .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-i\fR, \fB\-\-individual\fR Build all profiles separately. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Do not remove input's dir info for output. .TP \fB\-m\fR, \fB\-\-nomerged\fR Do not create a merged image of all profiles. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output file or directory name. .TP \fB\-\-psfinimg\fR PSF profiles made with all in output image. .TP \fB\-s\fR, \fB\-\-oversample\fR=\fI\,INT\/\fR Scale of oversampling. .TP \fB\-T\fR, \fB\-\-type\fR=\fI\,STR\/\fR byte, short, long, longlong, float, double. .TP \fB\-x\fR, \fB\-\-naxis1\fR=\fI\,INT\/\fR Number of pixels along first FITS axis. .TP \fB\-y\fR, \fB\-\-naxis2\fR=\fI\,INT\/\fR Number of pixels along second FITS axis. .IP Profiles: .TP \fB\-c\fR, \fB\-\-prepforconv\fR Shift and expand based on first catalog PSF. .TP \fB\-e\fR, \fB\-\-envseed\fR Use GSL_RNG_SEED environment variable for seed. .TP \fB\-\-magatpeak\fR Magnitude is for peak pixel, not full profile. .TP \fB\-p\fR, \fB\-\-tunitinp\fR Truncation is in units of pixels, not radius. .TP \fB\-r\fR, \fB\-\-numrandom\fR=\fI\,INT\/\fR No. of random points in Monte Carlo integration. .TP \fB\-R\fR, \fB\-\-replace\fR Replace overlapping profile pixels, don't add. .TP \fB\-t\fR, \fB\-\-tolerance\fR=\fI\,FLT\/\fR Tolerance to switch to less accurate method. .TP \fB\-w\fR, \fB\-\-circumwidth\fR=\fI\,FLT\/\fR Width of circumference (inward) profiles .TP \fB\-X\fR, \fB\-\-xshift\fR=\fI\,FLT\/\fR Shift profile centers and enlarge image, X axis. .TP \fB\-Y\fR, \fB\-\-yshift\fR=\fI\,FLT\/\fR Shift profile centers and enlarge image, Y axis. .TP \fB\-z\fR, \fB\-\-zeropoint\fR=\fI\,FLT\/\fR Magnitude zero point. .IP Catalog (column number, starting from zero): .TP \fB\-\-deccol\fR=\fI\,INT\/\fR Center declination. .TP \fB\-\-fcol\fR=\fI\,INT\/\fR Sersic (0), Moffat (1), Gaussian (2), Point (3), Flat (4), Circumference (5). .TP \fB\-F\fR, \fB\-\-mforflatpix\fR mcol is flat pixel value (when f is 4 or 5) .TP \fB\-\-mcol\fR=\fI\,INT\/\fR Magnitude. .TP \fB\-\-ncol\fR=\fI\,INT\/\fR Sersic index or Moffat beta. .TP \fB\-\-pcol\fR=\fI\,INT\/\fR Position angle. .TP \fB\-\-qcol\fR=\fI\,INT\/\fR Axis ratio. .TP \fB\-\-racol\fR=\fI\,INT\/\fR Center right ascension. .TP \fB\-\-rcol\fR=\fI\,INT\/\fR Effective radius or FWHM in pixels. .TP \fB\-\-tcol\fR=\fI\,INT\/\fR Truncation in units of \fB\-\-rcol\fR, unless \fB\-\-tunitinp\fR. .TP \fB\-\-xcol\fR=\fI\,INT\/\fR Center along first FITS axis (horizontal). .TP \fB\-\-ycol\fR=\fI\,INT\/\fR Center along second FITS axis (vertical). .IP WCS parameters: .TP \fB\-\-crpix1\fR=\fI\,FLT\/\fR Pixel coordinate of reference point (axis 1). .TP \fB\-\-crpix2\fR=\fI\,FLT\/\fR Pixel coordinate of reference point (axis 2). .TP \fB\-\-crval1\fR=\fI\,FLT\/\fR Right ascension at reference point (degrees). .TP \fB\-\-crval2\fR=\fI\,FLT\/\fR Declination at reference point (degrees). .TP \fB\-\-resolution\fR=\fI\,FLT\/\fR Resolution of image (arcseconds/pixel). .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for MakeProfiles. .TP \fB\-\-nolog\fR No log file for programs which make one. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlydirconf\fR Only read current directory configuration file. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is this. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH AUTHOR Written by Mohammad Akhlaghi .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2016, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .SH "SEE ALSO" The full documentation for .B MakeProfiles is maintained as a Texinfo manual. If the .B info and .B MakeProfiles programs are properly installed at your site, the command .IP .B info MakeProfiles .PP should give you access to the complete manual. gnuastro-0.2.33-8a3b/doc/man/astmknoise.10000644000175000017500000000654613004464676014721 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.3. .TH MAKENOISE "1" "October 2016" "GNU Astronomy Utilities 0.2.33-8a3b" "User Commands" .SH NAME MakeNoise \- add noise to an image .SH SYNOPSIS .B astmknoise [\fI\,OPTION\/\fR...] \fI\,ASTRdata \/\fR... .SH DESCRIPTION MakeNoise is part of GNU Astronomy Utilities 0.2.33\-8a3b. MakeNoise will add noise to all the pixels in an input image. The noise parameters can be specified with the command line options. .PP For more information, please run any of the following commands. They will respectively show you the `Invoking MakeNoise' subsection, the complete `MakeNoise' section, or the full GNU Astronomy Utilities manual. In particular the first contains a very complete explanation of each option. .IP info astmknoise .IP info MakeNoise .IP info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP info help\-gnuastro .PP MakeNoise options: .IP Input: .TP \fB\-b\fR, \fB\-\-background\fR=\fI\,FLT\/\fR Fixed background magnitude for the image. .TP \fB\-e\fR, \fB\-\-envseed\fR Use GSL_RNG_SEED environment variable for seed. .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR Extension name or number of input data. .TP \fB\-s\fR, \fB\-\-stdadd\fR=\fI\,FLT\/\fR Standard deviation addition constant. .TP \fB\-z\fR, \fB\-\-zeropoint\fR=\fI\,FLT\/\fR Image zeropoint magnitude. .IP Output: .TP \fB\-d\fR, \fB\-\-doubletype\fR Save output as a double precision floating point. .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Do not remove input's dir info for output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output file or directory name. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for MakeNoise. .TP \fB\-\-nolog\fR No log file for programs which make one. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlydirconf\fR Only read current directory configuration file. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is this. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH AUTHOR Written by Mohammad Akhlaghi .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2016, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .SH "SEE ALSO" The full documentation for .B MakeNoise is maintained as a Texinfo manual. If the .B info and .B MakeNoise programs are properly installed at your site, the command .IP .B info MakeNoise .PP should give you access to the complete manual. gnuastro-0.2.33-8a3b/doc/man/astmkcatalog.10000644000175000017500000001672413004464676015215 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.3. .TH MAKECATALOG "1" "October 2016" "GNU Astronomy Utilities 0.2.33-8a3b" "User Commands" .SH NAME MakeCatalog \- Make a catalog from labeled input images .SH SYNOPSIS .B astmkcatalog [\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR .SH DESCRIPTION MakeCatalog is part of GNU Astronomy Utilities 0.2.33\-8a3b. MakeCatalog will create a catalog from an input, labeled, and noise identification images. .PP For more information, please run any of the following commands. They will respectively show you the `Invoking MakeCatalog' subsection, the complete `MakeCatalog' section, or the full GNU Astronomy Utilities manual. In particular the first contains a very complete explanation of each option. .IP info astmkcatalog .IP info MakeCatalog .IP info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP info help\-gnuastro .PP MakeCatalog options: .IP Input: .TP \fB\-c\fR, \fB\-\-clumplabs\fR=\fI\,STR\/\fR Image specifying clump labels. .TP \fB\-\-clumphdu\fR=\fI\,STR\/\fR Clumps image header name or number. .TP \fB\-E\fR, \fB\-\-skysubtracted\fR Input is already sky subtracted (for S/N). .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR Extension name or number of input data. .TP \fB\-H\fR, \fB\-\-mhdu\fR=\fI\,STR\/\fR Mask image header name or number. .TP \fB\-M\fR, \fB\-\-mask\fR=\fI\,STR\/\fR Mask image file name. .TP \fB\-\-objhdu\fR=\fI\,STR\/\fR Object image header name or number. .TP \fB\-O\fR, \fB\-\-objlabs\fR=\fI\,STR\/\fR Image specifying object labels. .TP \fB\-s\fR, \fB\-\-skyfilename\fR=\fI\,STR\/\fR Sky value image. .TP \fB\-\-skyhdu\fR=\fI\,STR\/\fR Sky image header name or number. .TP \fB\-\-stdhdu\fR=\fI\,STR\/\fR Sky STD image header name or number. .TP \fB\-t\fR, \fB\-\-stdfilename\fR=\fI\,STR\/\fR Sky standard deviation image. .TP \fB\-T\fR, \fB\-\-threshold\fR=\fI\,FLT\/\fR Only values larger than this multiple of STD. .TP \fB\-z\fR, \fB\-\-zeropoint\fR=\fI\,FLT\/\fR Image zeropoint magnitude. .IP Output: .TP \fB\-\-accuprecision\fR=\fI\,INT\/\fR Precision of more accurate floating pnt. cols. .TP \fB\-\-accuwidth\fR=\fI\,INT\/\fR Width of more accurate floating point columns. .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-\-floatprecision\fR=\fI\,INT\/\fR Precision of floating point columns. .TP \fB\-\-floatwidth\fR=\fI\,INT\/\fR Width of floating point columns. .TP \fB\-\-intwidth\fR=\fI\,INT\/\fR Width of integer columns. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Do not remove input's dir info for output. .TP \fB\-\-nsigmag\fR=\fI\,FLT\/\fR Multiple of Sky STD to report magnitude of. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output file or directory name. .IP Upper limit magnitude: .TP \fB\-\-envseed\fR Random number generator info from environment. .TP \fB\-\-upmask\fR=\fI\,STR\/\fR Mask image file name only for upper limit. .TP \fB\-\-upmaskhdu\fR=\fI\,STR\/\fR Upper limit mask image header name or number. .TP \fB\-\-upnsigma\fR=\fI\,FLT\/\fR Multiple of final sigma to use. .TP \fB\-\-upnum\fR=\fI\,INT\/\fR Number of randomly positioned samples. .TP \fB\-\-upsclipaccu\fR=\fI\,FLT\/\fR Acceptable relative diff to stop clipping. .TP \fB\-\-upsclipmultip\fR=\fI\,FLT\/\fR Sigma clipping multiple of std. .IP Catalog columns: .TP \fB\-a\fR, \fB\-\-area\fR Number of pixels. .TP \fB\-A\fR, \fB\-\-semimajor\fR Flux weighted Semi\-major axis. .TP \fB\-b\fR, \fB\-\-brightness\fR Brightness (sum of pixel values). .TP \fB\-B\fR, \fB\-\-semiminor\fR Flux weighted Semi\-minor axis. .TP \fB\-\-clumpbrightness\fR Brightness in clumps of an object. .TP \fB\-\-clumpsarea\fR Area of clumps in an object. .TP \fB\-\-clumpsdec\fR Clumps flux weighted center declination. .TP \fB\-\-clumpsgeodec\fR Clumps geometric center declination. .TP \fB\-\-clumpsgeora\fR Clumps geometric center right ascension. .TP \fB\-\-clumpsgeox\fR Clumps geometric center (first FITS axis). .TP \fB\-\-clumpsgeoy\fR Clumps geometric center (second FITS axis). .TP \fB\-\-clumpsmagnitude\fR Total magnitude of clumps in this object. .TP \fB\-\-clumpsra\fR Clumps flux weighted center right ascension. .TP \fB\-\-clumpsx\fR Clumps flux weighted center (first FITS axis). .TP \fB\-\-clumpsy\fR Clumps flux weighted center (second FITS axis). .TP \fB\-C\fR, \fB\-\-numclumps\fR Number of clumps in this object. .TP \fB\-d\fR, \fB\-\-dec\fR All object flux weighted center declination. .TP \fB\-e\fR, \fB\-\-magnitudeerr\fR Total magnitude error. .TP \fB\-\-geodec\fR All object geometric center declination. .TP \fB\-\-geopositionangle\fR Flux weighted Position angle. .TP \fB\-\-geora\fR All object geometric center right ascension. .TP \fB\-\-geosemimajor\fR Flux weighted Semi\-major axis. .TP \fB\-\-geosemiminor\fR Flux weighted Semi\-minor axis. .TP \fB\-\-geox\fR All obj. geometric center (first FITS axis). .TP \fB\-\-geoy\fR All obj. geometric center (second FITS axis). .TP \fB\-i\fR, \fB\-\-id\fR Overall ID of this object or clump. .TP \fB\-I\fR, \fB\-\-idinhostobj\fR ID of clump in host object. .TP \fB\-j\fR, \fB\-\-hostobjid\fR ID of object hosting this clump. .TP \fB\-m\fR, \fB\-\-magnitude\fR Total magnitude. .TP \fB\-\-noriverbrightness\fR Sky (not river) subtracted clump brightness. .TP \fB\-n\fR, \fB\-\-sn\fR Signal to noise ratio column. .TP \fB\-p\fR, \fB\-\-positionangle\fR Flux weighted Position angle. .TP \fB\-r\fR, \fB\-\-ra\fR All object flux weighted center right ascension. .TP \fB\-\-riverave\fR Average river value surrounding this clump. .TP \fB\-\-rivernum\fR Number of river pixels surrounding this clump. .TP \fB\-\-sky\fR Sky value. .TP \fB\-\-std\fR Sky standard deviation. .TP \fB\-\-upperlimitmag\fR Upper limit magnitude for each clump or object. .TP \fB\-x\fR, \fB\-\-x\fR All obj. flux weighted center (first FITS axis). .TP \fB\-y\fR, \fB\-\-y\fR All obj. flux weighted center (second FITS axis). .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for MakeCatalog. .TP \fB\-\-nolog\fR No log file for programs which make one. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlydirconf\fR Only read current directory configuration file. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is this. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH AUTHOR Written by Mohammad Akhlaghi .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2016, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .SH "SEE ALSO" The full documentation for .B MakeCatalog is maintained as a Texinfo manual. If the .B info and .B MakeCatalog programs are properly installed at your site, the command .IP .B info MakeCatalog .PP should give you access to the complete manual. gnuastro-0.2.33-8a3b/doc/man/astimgwarp.10000644000175000017500000001035213004464676014710 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.3. .TH IMAGEWARP "1" "October 2016" "GNU Astronomy Utilities 0.2.33-8a3b" "User Commands" .SH NAME ImageWarp \- warp (transform) input image .SH SYNOPSIS .B astimgwarp [\fI\,OPTION\/\fR...] [\fI\,matrix.txt\/\fR] \fI\,ASTRdata \/\fR... .SH DESCRIPTION ImageWarp is part of GNU Astronomy Utilities 0.2.33\-8a3b. ImageWarp will warp/transform the input image using an input coordinate matrix. Currently it accepts any general projective mapping (which includes affine mappings as a subset). .PP For more information, please run any of the following commands. They will respectively show you the `Invoking ImageWarp' subsection, the complete `ImageWarp' section, or the full GNU Astronomy Utilities manual. In particular the first contains a very complete explanation of each option. .IP info astimgwarp .IP info ImageWarp .IP info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP info help\-gnuastro .PP ImageWarp options: .IP Input: .TP \fB\-\-hendwcs\fR=\fI\,INT\/\fR Header keyword number to stop reading WCS. .TP \fB\-\-hstartwcs\fR=\fI\,INT\/\fR Header keyword number to start reading WCS. .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR Extension name or number of input data. .TP \fB\-m\fR, \fB\-\-matrix\fR=\fI\,STR\/\fR Warp/Transform matrix elements. .TP \fB\-\-nofitscorrect\fR Do not shift to correct for FITS positioning. .IP Output: .TP \fB\-b\fR, \fB\-\-maxblankfrac\fR=\fI\,FLT\/\fR Maximum fraction of area covered by blank. .TP \fB\-d\fR, \fB\-\-doubletype\fR Do not convert output to input image type. .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Do not remove input's dir info for output. .TP \fB\-n\fR, \fB\-\-nowcscorrection\fR Do not correct input image WCS. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output file or directory name. .TP \fB\-z\fR, \fB\-\-zerofornoinput\fR Set pixels with no input to zero not blank. .IP Modular warpings: .TP \fB\-a\fR, \fB\-\-align\fR Align the image and celestial axes. .TP \fB\-e\fR, \fB\-\-shear\fR=\fI\,FLT[\/\fR,FLT] Shear along the given axis(es). .TP \fB\-f\fR, \fB\-\-flip\fR=\fI\,FLT[\/\fR,FLT] Flip along the given axis(es). .TP \fB\-p\fR, \fB\-\-project\fR=\fI\,FLT[\/\fR,FLT] Project along the given axis(es). .TP \fB\-r\fR, \fB\-\-rotate\fR=\fI\,FLT\/\fR Rotate by the given angle in degrees. .TP \fB\-s\fR, \fB\-\-scale\fR=\fI\,FLT[\/\fR,FLT] Scale along the given axis(es). .TP \fB\-t\fR, \fB\-\-translate\fR=\fI\,FLT[\/\fR,FLT] Translate along the given axis(es). .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for ImageWarp. .TP \fB\-\-nolog\fR No log file for programs which make one. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlydirconf\fR Only read current directory configuration file. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is this. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH AUTHOR Written by Mohammad Akhlaghi .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2016, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .SH "SEE ALSO" The full documentation for .B ImageWarp is maintained as a Texinfo manual. If the .B info and .B ImageWarp programs are properly installed at your site, the command .IP .B info ImageWarp .PP should give you access to the complete manual. gnuastro-0.2.33-8a3b/doc/man/astimgstat.10000644000175000017500000001264013004464676014714 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.3. .TH IMAGESTATISTICS "1" "October 2016" "GNU Astronomy Utilities 0.2.33-8a3b" "User Commands" .SH NAME ImageStatistics \- get image statistics .SH SYNOPSIS .B astimgstat [\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR .SH DESCRIPTION ImageStatistics is part of GNU Astronomy Utilities 0.2.33\-8a3b. ImageStatistics will print the basic statistics of the input image pixel flux distribution. All blank pixels or pixels specified by a mask image will be ignored. .PP For more information, please run any of the following commands. They will respectively show you the `Invoking ImageStatistics' subsection, the complete `ImageStatistics' section, or the full GNU Astronomy Utilities manual. In particular the first contains a very complete explanation of each option. .IP info astimgstat .IP info ImageStatistics .IP info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP info help\-gnuastro .PP ImageStatistics options: .IP Input: .TP \fB\-d\fR, \fB\-\-mirrordist\fR=\fI\,FLT\/\fR Distance beyond mirror point. Multiple of std. .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR Extension name or number of input data. .TP \fB\-H\fR, \fB\-\-mhdu\fR=\fI\,STR\/\fR Mask image header name. .TP \fB\-M\fR, \fB\-\-mask\fR=\fI\,STR\/\fR Mask image file name. .TP \fB\-r\fR, \fB\-\-ignoremin\fR Ignore data with values equal to minimum. .IP Output: .TP \fB\-A\fR, \fB\-\-noasciihist\fR Do not show an ASCII histogram of the data. .TP \fB\-B\fR, \fB\-\-onebinvalue\fR=\fI\,FLT\/\fR Shift bins so one bin starts on this value. .TP \fB\-\-checkmode\fR Mode mirror plot. `_modehist.txt', `_modecfp.txt' .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-\-histrangeformirror\fR Use input histogram range for mirror plots. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Do not remove input's dir info for output. .TP \fB\-l\fR, \fB\-\-lowerbin\fR Interval lower limit for column 1. .TP \fB\-\-mirrorplotdist\fR=\fI\,FLT\/\fR Distance beyond mode to display. .TP \fB\-\-mirrorquant\fR=\fI\,FLT\/\fR Mirror quantile. `_mirhist.txt', `_mircfp.txt'. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output file or directory name. .IP Histogram (suffix: `_hist.txt'): .TP \fB\-i\fR, \fB\-\-histmin\fR=\fI\,FLT\/\fR The minimum value for the histogram. .TP \fB\-\-maxhistone\fR Scale such that the maximum bin has value of one. .TP \fB\-\-nohist\fR Do not calculate histogram. .TP \fB\-\-normhist\fR Normalize the histogram (sum of all bins 1). .TP \fB\-n\fR, \fB\-\-histnumbins\fR=\fI\,INT\/\fR Number of bins in the histogram. .TP \fB\-Q\fR, \fB\-\-histquant\fR=\fI\,FLT\/\fR Quantile (Q) range. Histogram from Q to 1\-Q. .TP \fB\-x\fR, \fB\-\-histmax\fR=\fI\,FLT\/\fR The maximum value for the histogram. .IP Cumulative Frequency Plot (suffix: `_cfp.txt'): .TP \fB\-a\fR, \fB\-\-cfpmin\fR=\fI\,FLT\/\fR Minimum value to use in the CFP. .TP \fB\-b\fR, \fB\-\-cfpmax\fR=\fI\,FLT\/\fR Maximum value to use in the CFP. .TP \fB\-\-cfpsimhist\fR Set CFP range and bins similar to histogram. .TP \fB\-\-maxcfpeqmaxhist\fR Set maximum of CFP to maximum of histogram. .TP \fB\-\-nocfp\fR No Cumulative Frequency Plot. .TP \fB\-\-normcfp\fR Normalize the CFP (sum of all bins 1). .TP \fB\-p\fR, \fB\-\-cfpnum\fR=\fI\,INT\/\fR Number of data points to find CFP. .TP \fB\-U\fR, \fB\-\-cfpquant\fR=\fI\,FLT\/\fR Quantile of range: from U to 1\-U. .IP Sigma clipping: .TP \fB\-g\fR, \fB\-\-sigclipnum\fR=\fI\,INT\/\fR Number of times to do sigma clipping. .TP \fB\-\-nosigclip\fR Do not preform sigma clipping. .HP \fB\-t\fR, \fB\-\-sigcliptolerance\fR=\fI\,FLT\/\fR Difference in STD tolerance to halt iteration. .TP \fB\-u\fR, \fB\-\-sigclipmultip\fR=\fI\,FLT\/\fR Multiple of standard deviation in sigma\-clipping. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for ImageStatistics. .TP \fB\-\-nolog\fR No log file for programs which make one. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlydirconf\fR Only read current directory configuration file. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is this. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH AUTHOR Written by Mohammad Akhlaghi .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2016, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .SH "SEE ALSO" The full documentation for .B ImageStatistics is maintained as a Texinfo manual. If the .B info and .B ImageStatistics programs are properly installed at your site, the command .IP .B info ImageStatistics .PP should give you access to the complete manual. gnuastro-0.2.33-8a3b/doc/man/astimgcrop.10000644000175000017500000001165213004464676014706 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.3. .TH IMAGECROP "1" "October 2016" "GNU Astronomy Utilities 0.2.33-8a3b" "User Commands" .SH NAME ImageCrop \- crop regions of an image .SH SYNOPSIS .B astimgcrop [\fI\,OPTION\/\fR...] [\fI\,ASCIIcatalog\/\fR] \fI\,ASTRdata \/\fR... .SH DESCRIPTION ImageCrop is part of GNU Astronomy Utilities 0.2.33\-8a3b. ImageCrop will create cutouts, thumbnails, postage stamps or crops of region(s) from input image(s) using image or celestial coordinates. If muliple crops are desired, a catalog must be provided. When in WCS mode, if the cut out covers more than one input image, all overlapping input images will be stitched in the output. .PP For more information, please run any of the following commands. They will respectively show you the `Invoking ImageCrop' subsection, the complete `ImageCrop' section, or the full GNU Astronomy Utilities manual. In particular the first contains a very complete explanation of each option. .IP info astimgcrop .IP info ImageCrop .IP info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP info help\-gnuastro .PP ImageCrop options: .IP Input: .TP \fB\-\-hendwcs\fR=\fI\,INT\/\fR Header keyword number to stop reading WCS. .TP \fB\-\-hstartwcs\fR=\fI\,INT\/\fR Header keyword number to start reading WCS. .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR Extension name or number of input data. .IP Output: .TP \fB\-b\fR, \fB\-\-noblank\fR Remove parts of the crop box out of input image. .TP \fB\-c\fR, \fB\-\-checkcenter\fR=\fI\,INT\/\fR Side of box (in pixels) to check. .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-k\fR, \fB\-\-keepblankcenter\fR Keep crop if the central parts are not filled. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Do not remove input's dir info for output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output file or directory name. .TP \fB\-p\fR, \fB\-\-suffix\fR=\fI\,STR\/\fR Suffix (postfix) of cropped images. .IP Crop: .TP \fB\-a\fR, \fB\-\-iwidth\fR=\fI\,INT\/\fR Image mode width (in pixels). .TP \fB\-d\fR, \fB\-\-dec\fR=\fI\,FLT\/\fR Declination of one crop box center. .TP \fB\-f\fR, \fB\-\-racol\fR=\fI\,INT\/\fR Column of Right Ascension (RA) in catalog. .TP \fB\-g\fR, \fB\-\-deccol\fR=\fI\,INT\/\fR Column of Declination (Dec) in catalog. .TP \fB\-i\fR, \fB\-\-xcol\fR=\fI\,INT\/\fR Column of X (first FITS axis) value in catalog. .TP \fB\-j\fR, \fB\-\-ycol\fR=\fI\,INT\/\fR Column of Y (second FITS axis) in catalog. .TP \fB\-l\fR, \fB\-\-polygon\fR=\fI\,STR\/\fR Polygon vertices of region to crop. .TP \fB\-\-outpolygon\fR Keep the polygon's outside, mask the inside. .TP \fB\-r\fR, \fB\-\-ra\fR=\fI\,FLT\/\fR Right ascension of one crop box center. .TP \fB\-s\fR, \fB\-\-section\fR=\fI\,STR\/\fR Image section string specifying crop range. .TP \fB\-w\fR, \fB\-\-wwidth\fR=\fI\,FLT\/\fR WCS mode width (in arc seconds). .TP \fB\-x\fR, \fB\-\-xc\fR=\fI\,FLT\/\fR First axis position for only one crop. .TP \fB\-y\fR, \fB\-\-yc\fR=\fI\,FLT\/\fR Second axis position for only one crop. .TP \fB\-z\fR, \fB\-\-zeroisnotblank\fR 0.0 in float or double images are not blank. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for ImageCrop. .TP \fB\-I\fR, \fB\-\-imgmode\fR Use image coordinates (x and y). .TP \fB\-\-nolog\fR No log file for programs which make one. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlydirconf\fR Only read current directory configuration file. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is this. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .TP \fB\-W\fR, \fB\-\-wcsmode\fR Use WCS coordinates (Ra and Dec). .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH AUTHOR Written by Mohammad Akhlaghi .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2016, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .SH "SEE ALSO" The full documentation for .B ImageCrop is maintained as a Texinfo manual. If the .B info and .B ImageCrop programs are properly installed at your site, the command .IP .B info ImageCrop .PP should give you access to the complete manual. gnuastro-0.2.33-8a3b/doc/man/astheader.10000644000175000017500000000730513004464676014476 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.3. .TH HEADER "1" "October 2016" "GNU Astronomy Utilities 0.2.33-8a3b" "User Commands" .SH NAME Header \- view and manipulate FITS headers .SH SYNOPSIS .B astheader [\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR .SH DESCRIPTION Header is part of GNU Astronomy Utilities 0.2.33\-8a3b. Header print the header information in any astronomical data fileheader. It can also manipulate (add, remove or modify) any of the existing keywords in a data header. .PP For more information, please run any of the following commands. They will respectively show you the `Invoking Header' subsection, the complete `Header' section, or the full GNU Astronomy Utilities manual. In particular the first contains a very complete explanation of each option. .IP info astheader .IP info Header .IP info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP info help\-gnuastro .PP Header options: .IP Input: .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR Extension name or number of input data. .IP Output: .TP \fB\-a\fR, \fB\-\-asis\fR=\fI\,STR\/\fR Write the argument string as is into the header. .TP \fB\-c\fR, \fB\-\-comment\fR=\fI\,STR\/\fR Add COMMENT keyword, any length is ok. .TP \fB\-d\fR, \fB\-\-delete\fR=\fI\,STR\/\fR Delete a keyword from the header. .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-H\fR, \fB\-\-history\fR=\fI\,STR\/\fR Add HISTORY keyword, any length is ok. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Do not remove input's dir info for output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output file or directory name. .TP \fB\-r\fR, \fB\-\-rename\fR=\fI\,STR\/\fR Rename keyword, keeping value and comments. .TP \fB\-t\fR, \fB\-\-date\fR Set the DATE keyword to the current time. .TP \fB\-u\fR, \fB\-\-update\fR=\fI\,STR\/\fR Update a keyword value or comments. .TP \fB\-w\fR, \fB\-\-write\fR=\fI\,STR\/\fR Write a keyword (with value, comments and units). .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for Header. .TP \fB\-\-nolog\fR No log file for programs which make one. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlydirconf\fR Only read current directory configuration file. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is this. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-Q\fR, \fB\-\-quitonerror\fR Quit if there is an error on any action. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH AUTHOR Written by Mohammad Akhlaghi .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2016, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .SH "SEE ALSO" The full documentation for .B Header is maintained as a Texinfo manual. If the .B info and .B Header programs are properly installed at your site, the command .IP .B info Header .PP should give you access to the complete manual. gnuastro-0.2.33-8a3b/doc/man/astcosmiccal.10000644000175000017500000000701613004464676015202 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.3. .TH COSMICCALCULATOR "1" "October 2016" "GNU Astronomy Utilities 0.2.33-8a3b" "User Commands" .SH NAME CosmicCalculator \- estimate cosmological values .SH SYNOPSIS .B astcosmiccal [\fI\,OPTION\/\fR...] .SH DESCRIPTION CosmicCalculator is part of GNU Astronomy Utilities 0.2.33\-8a3b. CosmicCalculator will produce cosmological calculations. .PP For more information, please run any of the following commands. They will respectively show you the `Invoking CosmicCalculator' subsection, the complete `CosmicCalculator' section, or the full GNU Astronomy Utilities manual. In particular the first contains a very complete explanation of each option. .IP info astcosmiccal .IP info CosmicCalculator .IP info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP info help\-gnuastro .PP CosmicCalculator options: .IP Input: .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR Extension name or number of input data. .TP \fB\-H\fR, \fB\-\-H0\fR=\fI\,FLT\/\fR Current expansion rate (Hubble constant). .TP \fB\-l\fR, \fB\-\-olambda\fR=\fI\,FLT\/\fR Current cosmological cst. dens. per crit. dens. .TP \fB\-m\fR, \fB\-\-omatter\fR=\fI\,FLT\/\fR Current matter density per critical density. .TP \fB\-r\fR, \fB\-\-oradiation\fR=\fI\,FLT\/\fR Current radiation density per critical density. .TP \fB\-z\fR, \fB\-\-redshift\fR=\fI\,FLT\/\fR Redshift of interest. .IP Output: .TP \fB\-a\fR, \fB\-\-onlyabsmagconv\fR Only print conversion to absolute magnitude. .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Do not remove input's dir info for output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output file or directory name. .TP \fB\-v\fR, \fB\-\-onlyvolume\fR Only print comoving volume in Mpc^3 .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for CosmicCalculator. .TP \fB\-\-nolog\fR No log file for programs which make one. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlydirconf\fR Only read current directory configuration file. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is this. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH AUTHOR Written by Mohammad Akhlaghi .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2016, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .SH "SEE ALSO" The full documentation for .B CosmicCalculator is maintained as a Texinfo manual. If the .B info and .B CosmicCalculator programs are properly installed at your site, the command .IP .B info CosmicCalculator .PP should give you access to the complete manual. gnuastro-0.2.33-8a3b/doc/man/astconvolve.10000644000175000017500000001027013004464676015074 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.3. .TH CONVOLVE "1" "October 2016" "GNU Astronomy Utilities 0.2.33-8a3b" "User Commands" .SH NAME Convolve \- convolve an image with a given kernel .SH SYNOPSIS .B astconvolve [\fI\,OPTION\/\fR...] \fI\,InputFile\/\fR .SH DESCRIPTION Convolve is part of GNU Astronomy Utilities 0.2.33\-8a3b. Convolve will convolve an input image with a given spatial kernel (image) in the spatial domain (no edge effects) or frequency domain. The latter suffers from edge effects, but can be much faster. .PP For more information, please run any of the following commands. They will respectively show you the `Invoking Convolve' subsection, the complete `Convolve' section, or the full GNU Astronomy Utilities manual. In particular the first contains a very complete explanation of each option. .IP info astconvolve .IP info Convolve .IP info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP info help\-gnuastro .PP Convolve options: .IP Input: .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR Extension name or number of input data. .TP \fB\-H\fR, \fB\-\-mhdu\fR=\fI\,STR\/\fR Mask image header name. .TP \fB\-k\fR, \fB\-\-kernel\fR=\fI\,STR\/\fR Name of kernel for convolution. .TP \fB\-M\fR, \fB\-\-mask\fR=\fI\,STR\/\fR Mask image file name. .TP \fB\-\-nokernelflip\fR Do not flip the kernel image. .TP \fB\-\-nokernelnorm\fR Do not normalize the kernel image. .TP \fB\-U\fR, \fB\-\-khdu\fR=\fI\,STR\/\fR HDU of kernel file. .IP Output: .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Do not remove input's dir info for output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output file or directory name. .TP \fB\-v\fR, \fB\-\-viewfreqsteps\fR View the steps in the frequency domain. .IP Mesh grid (only for spatial domain): .TP \fB\-a\fR, \fB\-\-nch1\fR=\fI\,INT\/\fR Number of channels along first FITS axis. .TP \fB\-b\fR, \fB\-\-nch2\fR=\fI\,INT\/\fR Number of channels along second FITS axis. .TP \fB\-\-checkmesh\fR Store mesh IDs in `_mesh.fits' file. .TP \fB\-\-fullconvolution\fR Ignore channels in imageconvolution. .TP \fB\-L\fR, \fB\-\-lastmeshfrac\fR=\fI\,INT\/\fR Fraction of last mesh area to add new. .TP \fB\-s\fR, \fB\-\-meshsize\fR=\fI\,INT\/\fR Size of each mesh (tile) in the grid. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for Convolve. .TP \fB\-f\fR, \fB\-\-frequency\fR Frequency domain convolution. .TP \fB\-m\fR, \fB\-\-makekernel\fR=\fI\,INT\/\fR Make 2*INT kernel to create input image. .TP \fB\-\-nolog\fR No log file for programs which make one. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlydirconf\fR Only read current directory configuration file. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is this. .TP \fB\-p\fR, \fB\-\-spatial\fR Spatial domain convolution. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH AUTHOR Written by Mohammad Akhlaghi .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2016, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .SH "SEE ALSO" The full documentation for .B Convolve is maintained as a Texinfo manual. If the .B info and .B Convolve programs are properly installed at your site, the command .IP .B info Convolve .PP should give you access to the complete manual. gnuastro-0.2.33-8a3b/doc/man/astconvertt.10000644000175000017500000001040513004464676015105 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.3. .TH CONVERTTYPE "1" "October 2016" "GNU Astronomy Utilities 0.2.33-8a3b" "User Commands" .SH NAME ConvertType \- convert known data types to each other .SH SYNOPSIS .B astconvertt [\fI\,OPTION\/\fR...] \fI\,InputFile1 \/\fR[\fI\,InputFile2\/\fR] ... [\fI\,InputFile4\/\fR] .SH DESCRIPTION ConvertType is part of GNU Astronomy Utilities 0.2.33\-8a3b. ConvertType will convert any of the known input formats to any other of the known formats. The output file will have the same number of pixels. .PP For more information, please run any of the following commands. They will respectively show you the `Invoking ConvertType' subsection, the complete `ConvertType' section, or the full GNU Astronomy Utilities manual. In particular the first contains a very complete explanation of each option. .IP info astconvertt .IP info ConvertType .IP info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP info help\-gnuastro .PP ConvertType options: .IP Input: .TP \fB\-\-hdu2\fR=\fI\,STR\/\fR HDU of second input FITS image. .TP \fB\-\-hdu3\fR=\fI\,STR\/\fR HDU of third input FITS image. .TP \fB\-\-hdu4\fR=\fI\,STR\/\fR HDU of fourth input FITS image. .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR Extension name or number of input data. .IP Output: .TP \fB\-b\fR, \fB\-\-borderwidth\fR=\fI\,FLT\/\fR Border width (EPS, PDF) in units of 1/72 inch. .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Do not remove input's dir info for output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output file or directory name. .TP \fB\-u\fR, \fB\-\-quality\fR=\fI\,INT\/\fR Quality of output JPEG image (1 to 100). .TP \fB\-w\fR, \fB\-\-widthincm\fR=\fI\,FLT\/\fR Width in units of centimeters. .TP \fB\-x\fR, \fB\-\-hex\fR Hexadecimal encoding in EPS. Default: ASCII85. .IP Flux: .TP \fB\-a\fR, \fB\-\-fhmaxbyte\fR Set value of fluxhigh as the maximum byte value. .TP \fB\-c\fR, \fB\-\-change\fR=\fI\,STR\/\fR Change pixel values `from_1:to_1,from_2:to_2`. .TP \fB\-C\fR, \fB\-\-changeaftertrunc\fR First truncate then change pixel values. .TP \fB\-H\fR, \fB\-\-fluxhigh\fR=\fI\,FLT\/\fR Higher flux truncation value. .TP \fB\-i\fR, \fB\-\-flminbyte\fR Set value of fluxlow as the minimum byte value. .TP \fB\-l\fR, \fB\-\-log\fR Save flux in log scale. .TP \fB\-L\fR, \fB\-\-fluxlow\fR=\fI\,FLT\/\fR Lower flux truncation value. .TP \fB\-m\fR, \fB\-\-maxbyte\fR=\fI\,INT\/\fR Maximum byte value for all color channels. .TP \fB\-n\fR, \fB\-\-noinvert\fR Don't invert the image. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for ConvertType. .TP \fB\-\-nolog\fR No log file for programs which make one. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlydirconf\fR Only read current directory configuration file. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is this. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH AUTHOR Written by Mohammad Akhlaghi .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2016, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .SH "SEE ALSO" The full documentation for .B ConvertType is maintained as a Texinfo manual. If the .B info and .B ConvertType programs are properly installed at your site, the command .IP .B info ConvertType .PP should give you access to the complete manual. gnuastro-0.2.33-8a3b/doc/man/astarithmetic.10000644000175000017500000001012313004464676015367 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.3. .TH ARITHMETIC "1" "October 2016" "GNU Astronomy Utilities 0.2.33-8a3b" "User Commands" .SH NAME Arithmetic \- arithmetic operations on images and numbers .SH SYNOPSIS .B astarithmetic [\fI\,OPTION\/\fR...] \fI\,ASTRdata or number \/\fR[\fI\,ASTRdata\/\fR] \fI\,OPERATOR \/\fR... .SH DESCRIPTION Arithmetic is part of GNU Astronomy Utilities 0.2.33\-8a3b. Arithmetic will do arithmetic operations on one or multiple images and numbers. Simply put, the name of the image along with the arithmetic operators and possible numbers are given as arguments. The extensions of each input image are expected as options (starting with `hdu') listed below. Please note that currently Arithmetic only supports postfix or reverse polish notation. For example to get the result of `5+6', you should write `5 6 +', or to get the average of two images, you should write `a.fits b.fits + 2 /' (or more simply a.fits b.fits average). Please see the manual for more information. .PP The operators/functions recognized by Arithmetic are: +, \-, *, /, abs, pow, sqrt, log, log10, minvalue, maxvalue, min, max, average, median, lt, le, gt, ge, eq, neq, and, or, not, isblank. Please run `info gnuastro "Arithmetic operators"' for detailed information on each operator. Note that multiplication should be quoted (like "*", or '*') to avoid shell expansion. .PP For more information, please run any of the following commands. They will respectively show you the `Invoking Arithmetic' subsection, the complete `Arithmetic' section, or the full GNU Astronomy Utilities manual. In particular the first contains a very complete explanation of each option. .IP info astarithmetic .IP info Arithmetic .IP info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP info help\-gnuastro .PP Arithmetic options: .IP Input: .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR Nth call of this option, used for Nth input FITS. .TP \fB\-H\fR, \fB\-\-mhdu\fR=\fI\,STR\/\fR Mask image header name. .TP \fB\-M\fR, \fB\-\-mask\fR=\fI\,STR\/\fR Mask image file name. .IP Output: .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Do not remove input's dir info for output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output file or directory name. .TP \fB\-T\fR, \fB\-\-type\fR=\fI\,STR\/\fR byte, short, long, longlong, float, double. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for Arithmetic. .TP \fB\-\-nolog\fR No log file for programs which make one. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlydirconf\fR Only read current directory configuration file. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is this. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH AUTHOR Written by Mohammad Akhlaghi .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2016, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .SH "SEE ALSO" The full documentation for .B Arithmetic is maintained as a Texinfo manual. If the .B info and .B Arithmetic programs are properly installed at your site, the command .IP .B info Arithmetic .PP should give you access to the complete manual. gnuastro-0.2.33-8a3b/doc/gnuastro-figures/0000755000175000017500000000000013004464725015253 500000000000000gnuastro-0.2.33-8a3b/doc/gnuastro-figures/sphericalplane.txt0000644000175000017500000000005013004437012020706 00000000000000../gnuastro-figures//sphericalplane.eps gnuastro-0.2.33-8a3b/doc/gnuastro-figures/sphericalplane.png0000644000175000017500000003003213004437012020656 00000000000000‰PNG  IHDRʤk­}gAMA± üa cHRMz&€„ú€èu0ê`:˜pœºQ<bKGDÿ‡Ì¿ pHYs––qFþðtIMEà 0:‹u.ªIDATxÚí{”$WyØWK‹«tÁæHÔbˆÍÙläK²¤×€°6='–u°‚qm=,,ëôDB[QÒc" #èìe³d= ÁêŽ×zØ–œ©l–µ9¤éÕa@S+VBûÐróG×ÌôÌt÷ô£ºêÞªï7çìΣ·ºûWß½_}÷^¥ìDÕõTÚmÆÁIi7@„µˆ”‚`"¥ †H)†!R ‚aˆ”‚`"¥ †H)tE¹ª¬|PEUTNÚ­É"¥ÐU  g)¨y¸”ÒnO~8%íÆâéYšº©ši7'?()³³•dÊìÔ"³º–ö±æ é¾ =P.. 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Jones %Copyright: Copyright (c) 1997, 2009 American Mathematical Society %Copyright: (), with Reserved Font Name CMR7. % This Font Software is licensed under the SIL Open Font License, Version 1.1. % This license is in the accompanying file OFL.txt, and is also % available with a FAQ at: http://scripts.sil.org/OFL. %%EndComments FontDirectory/CMR7 known{/CMR7 findfont dup/UniqueID known{dup /UniqueID get 5000790 eq exch/FontType get 1 eq and}{pop false}ifelse {save true}{false}ifelse}{false}ifelse 11 dict begin /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0 ]readonly def /FontName /CMR7 def /FontBBox {-27 -250 1122 750 }readonly def /PaintType 0 def /FontInfo 9 dict dup begin /version (003.002) readonly def /Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050\051, with Reserved Font Name CMR7.) readonly def /FullName (CMR7) readonly def /FamilyName (Computer Modern) readonly def /Weight (Medium) readonly def /ItalicAngle 0 def /isFixedPitch false def 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Jones %Copyright: Copyright (c) 1997, 2009 American Mathematical Society %Copyright: (), with Reserved Font Name CMR10. % This Font Software is licensed under the SIL Open Font License, Version 1.1. % This license is in the accompanying file OFL.txt, and is also % available with a FAQ at: http://scripts.sil.org/OFL. %%EndComments FontDirectory/CMR10 known{/CMR10 findfont dup/UniqueID known{dup /UniqueID get 5000793 eq exch/FontType get 1 eq and}{pop false}ifelse {save true}{false}ifelse}{false}ifelse 11 dict begin /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0 ]readonly def /FontName /CMR10 def /FontBBox {-40 -250 1009 750 }readonly def /PaintType 0 def /FontInfo 9 dict dup begin /version (003.002) readonly def /Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050\051, with Reserved Font Name CMR10.) readonly def /FullName (CMR10) readonly def /FamilyName (Computer Modern) readonly def /Weight (Medium) readonly def /ItalicAngle 0 def /isFixedPitch false def 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377.00269 14.2253 lineto pgfstr restore save 0.19925 pgfw 337.32684 17.00824 moveto 337.32684 14.17339 lineto pgfstr save save [1.0 0.0 0.0 1.0 327.88268 5.93782 ] concat pgfs 0 setgray -596 414 a Fe(\000)p Ff(!)-497 422 y Fd(m)-596 414 y pgfr restore restore restore save 0.19925 pgfw 377.01265 17.00824 moveto 377.01265 14.17339 lineto pgfstr save save [1.0 0.0 0.0 1.0 367.56848 5.93782 ] concat pgfs 0 setgray -596 414 a Fg(+)p Ff(!)-497 422 y Fd(m)-596 414 y pgfr restore restore restore 357.16995 14.17339 moveto pgfstr save save [1.0 0.0 0.0 1.0 355.05284 5.51721 ] concat pgfs 0 setgray -596 414 a Fg(0)-596 414 y pgfr restore restore save [ 0.3985 1.99255 ] 0.0 setdash 331.65758 14.17339 moveto 331.65758 99.21382 lineto pgfstr restore save [ 0.3985 1.99255 ] 0.0 setdash 382.68192 14.17339 moveto 382.68192 99.21382 lineto pgfstr restore save 0.5 setgray 0.3985 pgfw 332.11584 90.7097 moveto 382.22363 90.7097 lineto pgfstr save [-1.0 0.0 0.0 -1.0 332.11584 90.7097 ] concat save 0.31879 pgfw [ ] 0.0 setdash 1 setlinecap 1 setlinejoin -1.19551 1.59401 moveto -1.09587 0.99626 0.0 0.09961 0.29886 0.0 curveto 0.0 -0.09961 -1.09587 -0.99626 -1.19551 -1.59401 curveto pgfstr restore restore save [1.0 0.0 0.0 1.0 382.22363 90.7097 ] concat save 0.31879 pgfw [ ] 0.0 setdash 1 setlinecap 1 setlinejoin -1.19551 1.59401 moveto -1.09587 0.99626 0.0 0.09961 0.29886 0.0 curveto 0.0 -0.09961 -1.09587 -0.99626 -1.19551 -1.59401 curveto pgfstr restore restore restore 357.16995 90.7097 moveto pgfstr save save [1.0 0.0 0.0 1.0 351.53423 97.66507 ] concat pgfs 0 setgray -586 381 a Fb(2)p Fc(\031)p -586 395 75 4 v -574 443 a(P)-596 414 y pgfr restore restore save 1.49442 pgfw 388.3512 14.17339 moveto 388.3512 14.22443 lineto 389.1609 14.26335 lineto 389.97061 14.32738 lineto 390.78033 14.43118 lineto 391.59003 14.59468 lineto 392.39975 14.84209 lineto 393.20946 15.21667 lineto 394.01918 15.7608 lineto 394.82887 16.53764 lineto 395.6386 17.60948 lineto 396.4483 19.04982 lineto 397.25801 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restore save 0.19925 pgfw 408.19388 17.00824 moveto 408.19388 14.17339 lineto pgfstr save save [1.0 0.0 0.0 1.0 398.64032 5.52275 ] concat pgfs 0 setgray -596 414 a Fb(2)p Fc(\031)r(=P)-596 414 y pgfr restore restore restore save 1.49442 pgfw 439.37553 14.17339 moveto 439.37553 14.22443 lineto 440.0118 14.25298 lineto 440.64807 14.29623 lineto 441.28433 14.35939 lineto 441.9206 14.45021 lineto 442.55685 14.58083 lineto 443.19312 14.76251 lineto 443.82938 15.01251 lineto 444.46565 15.35248 lineto 445.10191 15.81184 lineto 445.73817 16.41307 lineto 446.37444 17.1899 lineto 447.0107 18.1761 lineto 447.64696 19.41835 lineto 448.28323 20.93828 lineto 448.9195 22.7757 lineto 449.55576 24.9583 lineto 450.19202 27.49384 lineto 450.82828 30.39703 lineto 451.46454 33.64626 lineto 452.10081 37.21297 lineto 452.73708 41.04611 lineto 453.37334 45.06699 lineto 454.0096 49.18388 lineto 454.64586 53.27829 lineto 455.28214 57.23082 lineto 455.9184 60.8996 lineto 456.55466 64.16612 lineto 457.19092 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pgfstr grestore} bind def /pgf6{gsave exec 1.0 pgfw [ ] 0.0 setdash -4.50003 -5.00005 moveto 0.49998 0.0 lineto -4.50003 5.00005 lineto pgfstr grestore} bind def /pgf7{gsave exec 1.0 pgfw -2.50002 0.0 translate [ ] 0.0 setdash 3.00003 0.0 moveto 3.00003 1.65689 1.65689 3.00003 0.0 3.00003 curveto -1.65689 3.00003 -3.00003 1.65689 -3.00003 0.0 curveto -3.00003 -1.65689 -1.65689 -3.00003 0.0 -3.00003 curveto 1.65689 -3.00003 3.00003 -1.65689 3.00003 0.0 curveto closepath gsave pgffc pgffill grestore gsave pgfsc pgfstr grestore newpath grestore} bind def /pgf8{gsave exec 1.0 pgfw [ ] 0.0 setdash 1.0 0.0 moveto -5.00005 3.00003 lineto -11.00012 0.0 lineto -5.00005 -3.00003 lineto closepath gsave pgffc pgffill grestore gsave pgfsc pgfstr grestore newpath grestore} bind def @fedspecial end %%BeginFont: CMR5 %!PS-AdobeFont-1.0: CMR5 003.002 %%Title: CMR5 %Version: 003.002 %%CreationDate: Mon Jul 13 16:17:00 2009 %%Creator: David M. 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pgfr restore restore 162.7683 54.25609 moveto pgfstr save save [1.0 0.0 0.0 1.0 161.07321 47.52606 ] concat pgfs 0 setgray -596 432 a Fa(2)-596 432 y pgfr restore restore 177.56471 54.25609 moveto pgfstr save save [1.0 0.0 0.0 1.0 175.86963 47.52606 ] concat pgfs 0 setgray -596 432 a Fa(3)-596 432 y pgfr restore restore save 0.99628 pgfw 246.61725 0.0 moveto 246.61725 0.0 moveto 246.61725 123.30862 lineto 483.36772 123.30862 lineto 483.36772 0.0 lineto closepath 483.36772 123.30862 moveto pgfstr restore 249.08583 108.51219 moveto pgfstr save save [1.0 0.0 0.0 1.0 252.60565 112.03201 ] concat pgfs 0 setgray -596 432 a Fd(Time:)37 b(2sec)-596 432 y pgfr restore restore 256.48405 54.25609 moveto 344.80437 54.25609 lineto pgfstr save [1.0 0.0 0.0 1.0 344.80437 54.25609 ] concat save 0.31879 pgfw [ ] 0.0 setdash 1 setlinecap 1 setlinejoin -1.19551 1.59401 moveto -1.09587 0.99626 0.0 0.09961 0.29886 0.0 curveto 0.0 -0.09961 -1.09587 -0.99626 -1.19551 -1.59401 curveto pgfstr restore restore 345.26265 54.25609 moveto pgfstr save save [1.0 0.0 0.0 1.0 343.85327 46.12158 ] concat pgfs 0 setgray -596 432 a Fc(i)-596 432 y pgfr restore restore 300.87335 9.86678 moveto 300.87335 98.1871 lineto pgfstr save [0.0 1.0 -1.0 0.0 300.87335 98.1871 ] concat save 0.31879 pgfw [ ] 0.0 setdash 1 setlinecap 1 setlinejoin -1.19551 1.59401 moveto -1.09587 0.99626 0.0 0.09961 0.29886 0.0 curveto 0.0 -0.09961 -1.09587 -0.99626 -1.19551 -1.59401 curveto pgfstr restore restore 300.87335 98.64539 moveto pgfstr save save [1.0 0.0 0.0 1.0 304.39317 96.9019 ] concat pgfs 0 setgray -596 432 a Fb(Real\(signal\))-596 432 y pgfr restore restore 300.87335 54.25609 moveto 330.4662 54.25609 moveto 330.4662 70.59998 317.21724 83.84894 300.87335 83.84894 curveto 284.52946 83.84894 271.2805 70.59998 271.2805 54.25609 curveto 271.2805 37.91219 284.52946 24.66322 300.87335 24.66322 curveto 317.21724 24.66322 330.4662 37.91219 330.4662 54.25609 curveto closepath 300.87335 54.25609 moveto pgfstr 315.66978 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367.84863 54.25609 ] concat save 2.39107 pgfw [ ] 0.0 setdash 1 setlinecap 1 setlinejoin -3.52684 4.70245 moveto -3.23293 2.93903 0.0 0.2939 0.8817 0.0 curveto 0.0 -0.2939 -3.23293 -2.93903 -3.52684 -4.70245 curveto pgfstr restore restore restore save [ 2.98883 2.98883 ] 0.0 setdash 0.3985 pgfw 300.87335 69.99329 moveto 409.38554 69.99329 lineto pgfstr restore 374.85551 54.25609 moveto 473.05017 54.25609 lineto pgfstr save [1.0 0.0 0.0 1.0 473.05017 54.25609 ] concat save 0.31879 pgfw [ ] 0.0 setdash 1 setlinecap 1 setlinejoin -1.19551 1.59401 moveto -1.09587 0.99626 0.0 0.09961 0.29886 0.0 curveto 0.0 -0.09961 -1.09587 -0.99626 -1.19551 -1.59401 curveto pgfstr restore restore 473.50845 54.25609 moveto pgfstr save save [1.0 0.0 0.0 1.0 432.80656 45.50581 ] concat pgfs 0 setgray -596 432 a Fb(Time)22 b(\(sec\))-596 432 y pgfr restore restore 379.79268 9.86678 moveto 379.79268 98.1871 lineto pgfstr save [0.0 1.0 -1.0 0.0 379.79268 98.1871 ] concat save 0.31879 pgfw [ ] 0.0 setdash 1 setlinecap 1 setlinejoin -1.19551 1.59401 moveto -1.09587 0.99626 0.0 0.09961 0.29886 0.0 curveto 0.0 -0.09961 -1.09587 -0.99626 -1.19551 -1.59401 curveto pgfstr restore restore 379.79268 98.64539 moveto pgfstr save save [1.0 0.0 0.0 1.0 383.3125 96.9019 ] concat pgfs 0 setgray -596 432 a Fb(Real\(signal\))-596 432 y pgfr restore restore save /pgffc{0 setgray}def 394.58911 78.91931 moveto 395.58539 78.91931 moveto 395.58539 79.46954 395.13934 79.91559 394.58911 79.91559 curveto 394.03888 79.91559 393.59283 79.46954 393.59283 78.91931 curveto 393.59283 78.36908 394.03888 77.92303 394.58911 77.92303 curveto 395.13934 77.92303 395.58539 78.36908 395.58539 78.91931 curveto closepath 394.58911 78.91931 moveto gsave pgffc pgffill grestore gsave pgfsc pgfstr grestore newpath restore save /pgffc{0 setgray}def 409.38554 69.99329 moveto 410.38182 69.99329 moveto 410.38182 70.54353 409.93578 70.98956 409.38554 70.98956 curveto 408.83531 70.98956 408.38927 70.54353 408.38927 69.99329 curveto 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gnuastro-0.2.33-8a3b/bin/0000755000175000017500000000000013004464725011752 500000000000000gnuastro-0.2.33-8a3b/bin/table/0000755000175000017500000000000013004464725013041 500000000000000gnuastro-0.2.33-8a3b/bin/table/table.h0000644000175000017500000000205612757417261014233 00000000000000/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef TABLE_H #define TABLE_H void table(struct tableparams *p); #endif gnuastro-0.2.33-8a3b/bin/table/table.c0000644000175000017500000002626113004133440014206 00000000000000/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include "main.h" /**************************************************************/ /*************** Input table *******************/ /**************************************************************/ /* Set the format string for each column: */ void setformatstring(struct tableparams *p, size_t outcolid) { struct uiparams *up=&p->up; char width[10], accu[10], *type=NULL; struct outcolumn *ocol=&p->ocols[outcolid]; switch(ocol->datatype) { case TBIT: error(EXIT_FAILURE, 0, "Table doesn't print TBIT data type " "currently, please contact us at %s so we can implement " "it.", PACKAGE_BUGREPORT); case TBYTE: type="u"; sprintf(width, "%zu", up->sintwidth); accu[0]='\0'; break; case TLOGICAL: case TSBYTE: type="d"; sprintf(width, "%zu", up->sintwidth); accu[0]='\0'; break; case TSTRING: type="s"; if(up->sintwidth) sprintf(width, "%zu", up->sintwidth); else width[0]='\0'; accu[0]='\0'; break; case TSHORT: type="d"; sprintf(width, "%zu", up->sintwidth); accu[0]='\0'; break; case TLONG: type="ld"; sprintf(width, "%zu", up->lintwidth); accu[0]='\0'; break; case TLONGLONG: type="ld"; sprintf(width, "%zu", up->lintwidth); accu[0]='\0'; break; case TFLOAT: type = up->feg=='f' ? "f" : ( up->feg=='e' ? "e" : "g"); sprintf(width, "%zu", up->floatwidth); sprintf(accu, ".%zu", up->floatprecision); break; case TDOUBLE: type = up->feg=='f' ? "f" : ( up->feg=='e' ? "e" : "g"); sprintf(width, "%zu", up->doublewidth); sprintf(accu, ".%zu", up->doubleprecision); break; case TCOMPLEX: error(EXIT_FAILURE, 0, "Table doesn't print TCOMPLEX data type " "currently, please contact us at %s so we can implement " "it.", PACKAGE_BUGREPORT); break; case TDBLCOMPLEX: error(EXIT_FAILURE, 0, "Table doesn't print TDBLCOMPLEX data type " "currently, please contact us at %s so we can implement " "it.", PACKAGE_BUGREPORT); break; case TINT: type="d"; sprintf(width, "%zu", up->sintwidth); accu[0]='\0'; break; case TUINT: type="u"; sprintf(width, "%zu", up->sintwidth); accu[0]='\0'; break; case TUSHORT: type="u"; sprintf(width, "%zu", up->sintwidth); accu[0]='\0'; break; case TULONG: type="lu"; sprintf(width, "%zu", up->lintwidth); accu[0]='\0'; break; default: error(EXIT_FAILURE, 0, "datatype value of %d not recognized in " "setformatstring (table.c)", ocol->datatype); } /* Put the type, width and accu into the format string for this column: */ sprintf(ocol->fmt, "%%-%s%s%s", width, accu, type); } /* Read all the input columns */ void readinputcols(struct tableparams *p) { double *colfromtxt; struct outcolumn *col; int datatype, status=0; size_t i, j, nrows=p->nrows, incols=p->up.ncols; /* Get the contents of each table column: */ for(i=0;inocols;++i) { /* Variables for simple reading */ col=&p->ocols[i]; datatype=col->datatype; /* Allocate the blank value for this column. Note that we will also need the blankvalue for a text file when outputing to a FITS. */ col->nulval=gal_fits_datatype_blank(datatype); /* Read the input column. */ if(p->fitsptr) { /* Allocate space for the data in this column */ col->data=gal_fits_datatype_alloc(nrows, datatype); /* Call CFITSIO to read the column information. */ fits_read_col(p->fitsptr, datatype, col->inindex+1, 1, 1, nrows, col->nulval, col->data, &col->anynul, &status); } else { /* This is a text file, read by Gnuastro's current txtarray library. This library currently only reads a 2D table into a 2D array of type double. The important thing here is that the array is row-contiguous. But here we want column contiguous data. So we allocate an array to only put this column's values in.*/ errno=0; colfromtxt=col->data=malloc(nrows * col->esize); if(col->data==NULL) error(EXIT_FAILURE, errno, "%zu bytes for col->data", nrows * col->esize); for(j=0;jup.txtarray[ j * incols + col->inindex ]; } /* Set the format string to print the column values if the output is to be printed as text (either in a text file or to the standard output. */ if(p->outputtotxt || p->outputtostdout) setformatstring(p, i); } } /**************************************************************/ /*************** Output table *******************/ /**************************************************************/ void saveouttofits(struct tableparams *p) { size_t i; int status=0; fitsfile *fptr; struct uiparams *up=&p->up; char **ttype, **tform, **tunit; struct outcolumn *ocols=p->ocols; /* Allocate the information arrays for CFITSIO. */ errno=0; ttype=malloc(p->nocols*sizeof *ttype); if(ttype==NULL) error(EXIT_FAILURE, errno, "%zu bytes for ttype", p->nocols*sizeof *ttype); errno=0; tform=malloc(p->nocols*sizeof *tform); if(tform==NULL) error(EXIT_FAILURE, errno, "%zu bytes for tform", p->nocols*sizeof *tform); errno=0; tunit=malloc(p->nocols*sizeof *tunit); if(tunit==NULL) error(EXIT_FAILURE, errno, "%zu bytes for tunit", p->nocols*sizeof *tunit); /* Fill in the information arrays: */ for(i=0;inocols;++i) { tform[i]=up->ttstr[ ocols[i].inindex ]; ttype[i]=up->tname[ ocols[i].inindex ]; tunit[i]=up->tunit[ ocols[i].inindex ]; } /* Open the output FITS file. */ if(access(p->cp.output,F_OK) != -1 ) fits_open_file(&fptr, p->cp.output, READWRITE, &status); else fits_create_file(&fptr, p->cp.output, &status); /* Create a new table extension */ fits_create_tbl(fptr, p->fitstabletype, p->nrows, p->nocols, ttype, tform, tunit, "Table", &status); /* Write this column's data into the FITS file. */ for(i=0;inocols;++i) fits_write_colnull(fptr, ocols[i].datatype, i+1, 1, 1, p->nrows, ocols[i].data, ocols[i].nulval, &status); /* Include the ending comments and close the file. */ gal_fits_write_keys_version(fptr, NULL, SPACK_STRING); fits_close_file(fptr, &status); gal_fits_io_error(status, NULL); /* Clean up */ free(ttype); free(tform); free(tunit); } void printoutput(struct tableparams *p) { FILE *fp; size_t i, row; struct outcolumn *ocols=p->ocols; /* Determine the output stream and open the file for writing if its a file. */ if(p->outputtotxt) { errno=0; fp=fopen(p->cp.output, "w"); if(fp==NULL) error(EXIT_FAILURE, errno, "%s", p->cp.output); } else fp=stdout; /* Print each column and each row: */ for(row=0;rownrows;++row) { for(i=0;inocols;++i) switch(ocols[i].datatype) { case TBIT: error(EXIT_FAILURE, 0, "Table doesn't print TBIT data type " "currently, please contact us at %s so we can implement " "it.", PACKAGE_BUGREPORT); case TBYTE: fprintf(fp, ocols[i].fmt, ((unsigned char *)ocols[i].data)[row]); break; case TLOGICAL: case TSBYTE: fprintf(fp, ocols[i].fmt, ((char *)ocols[i].data)[row]); break; case TSTRING: fprintf(fp, ocols[i].fmt, ((char **)ocols[i].data)[row]); break; case TSHORT: fprintf(fp, ocols[i].fmt, ((short *)ocols[i].data)[row]); break; case TLONG: fprintf(fp, ocols[i].fmt, ((long *)ocols[i].data)[row]); break; case TLONGLONG: fprintf(fp, ocols[i].fmt, ((LONGLONG *)ocols[i].data)[row]); break; case TFLOAT: fprintf(fp, ocols[i].fmt, ((float *)ocols[i].data)[row]); break; case TDOUBLE: fprintf(fp, ocols[i].fmt, ((double *)ocols[i].data)[row]); break; case TCOMPLEX: error(EXIT_FAILURE, 0, "Table doesn't print TCOMPLEX data type " "currently, please contact us at %s so we can implement " "it.", PACKAGE_BUGREPORT); break; case TDBLCOMPLEX: error(EXIT_FAILURE, 0, "Table doesn't print TDBLCOMPLEX data " "type currently, please contact us at %s so we can " "implement it.", PACKAGE_BUGREPORT); break; case TINT: fprintf(fp, ocols[i].fmt, ((char *)ocols[i].data)[row]); break; case TUINT: fprintf(fp, ocols[i].fmt, ((unsigned int *)ocols[i].data)[row]); break; case TUSHORT: fprintf(fp, ocols[i].fmt, ((unsigned short *)ocols[i].data)[row]); break; case TULONG: fprintf(fp, ocols[i].fmt, ((unsigned long *)ocols[i].data)[row]); break; default: error(EXIT_FAILURE, 0, "datatype value of %d not recognized in " "printoutput", ocols[i].datatype); } fprintf(fp, "\n"); } /* If we printed to a file, then close it. */ if(p->outputtotxt) { errno=0; if( fclose(fp) == EOF ) error(EXIT_FAILURE, errno, "%s", p->cp.output); } } /**************************************************************/ /*************** Top function *******************/ /**************************************************************/ void table(struct tableparams *p) { readinputcols(p); if(p->outputtofits) saveouttofits(p); else printoutput(p); } gnuastro-0.2.33-8a3b/bin/table/args.h0000644000175000017500000001763112774161104014074 00000000000000/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef ARGS_H #define ARGS_H #include #include #include #include /**************************************************************/ /************** argp.h definitions ***************/ /**************************************************************/ /* Definition parameters for the argp: */ const char *argp_program_version=SPACK_STRING"\n"GAL_STRINGS_COPYRIGHT "\n\nWritten by Mohammad Akhlaghi"; const char *argp_program_bug_address=PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata"; const char doc[] = /* Before the list of options: */ GAL_STRINGS_TOP_HELP_INFO SPACK_NAME" prints (in a human readable format) a FITS table or its " "information. The output columns can either be selected by number, name " "or using regular expressions. The format of their printing can also " "be set (based on the type of data in the column).\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /* Available letters for short options: a b d e f g j k l m n p r s u v w x y z A B C E F G H J L M O Q R T U W X Y Z Number keys used: 1008 Options with keys (second structure element) larger than 500 do not have a short version. */ static struct argp_option options[] = { { 0, 0, 0, 0, "Input:", 1 }, { "column", 'c', "STR", 0, "Input column name, number or regular expression.", 1 }, { "ignorecase", 'I', 0, 0, "Ignore case when matching column names.", 1 }, { 0, 0, 0, 0, "Output:", 2 }, { "feg", 1001, "STR", 0, "`f': only decimals, `e': scientific, `g': either.", 2 }, { "sintwidth", 1002, "INT", 0, "Shorter integer column(s) width (num charachers).", 2 }, { "lintwidth", 1003, "INT", 0, "Longer integer column(s) width (num charachers).", 2 }, { "floatwidth", 1004, "INT", 0, "`float' column(s) width (num charachers).", 2 }, { "doublewidth", 1005, "INT", 0, "`double' column(s) width (num charachers).", 2 }, { "strwidth", 1006, "INT", 0, "String column(s) width (num charachers).", 2 }, { "floatprecision", 1007, "INT", 0, "`float' column(s) precision.", 2 }, { "doubleprecision", 1008, "INT", 0, "`double' column(s) precision.", 2 }, { "fitstabletype", 't', "STR", 0, "Only `ascii', or `binary' are acceptable.", 2 }, { 0, 0, 0, 0, "Operating modes:", -1 }, { "information", 'i', 0, 0, "Only print table and columns information.", -1 }, {0} }; /* Parse a single option: */ static error_t parse_opt(int key, char *arg, struct argp_state *state) { /* Save the arguments structure: */ char *tstring; struct tableparams *p = state->input; /* Set the pointer to the common parameters for all programs here: */ state->child_inputs[0]=&p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); switch(key) { /* Input: */ case 'c': gal_checkset_allocate_copy(arg, &tstring); gal_linkedlist_add_to_stll(&p->up.columns, tstring); break; case 'I': p->up.ignorecase=1; p->up.ignorecaseset=1; break; /* Output: */ case 1001: checksetfge(arg, &p->up.feg, NULL, 0); p->up.fegset=1; break; case 1002: gal_checkset_sizet_el_zero(arg, &p->up.sintwidth, "sintwidth", key, SPACK, NULL, 0); p->up.sintwidthset=1; break; case 1003: gal_checkset_sizet_el_zero(arg, &p->up.lintwidth, "lintwidth", key, SPACK, NULL, 0); p->up.lintwidthset=1; break; case 1004: gal_checkset_sizet_el_zero(arg, &p->up.floatwidth, "floatwidth", key, SPACK, NULL, 0); p->up.floatwidthset=1; break; case 1005: gal_checkset_sizet_el_zero(arg, &p->up.doublewidth, "doublewidth", key, SPACK, NULL, 0); p->up.doublewidthset=1; break; case 1006: gal_checkset_sizet_el_zero(arg, &p->up.strwidth, "strwidth", key, SPACK, NULL, 0); p->up.strwidthset=1; break; case 1007: gal_checkset_sizet_el_zero(arg, &p->up.floatprecision, "floatprecision", key, SPACK, NULL, 0); p->up.floatprecisionset=1; break; case 1008: gal_checkset_sizet_el_zero(arg, &p->up.doubleprecision, "doubleprecision", key, SPACK, NULL, 0); p->up.doubleprecisionset=1; break; case 't': checksetfitstabletype(arg, &p->up.feg, NULL, 0); p->up.fitstabletypeset=1; break; /* Operating modes: */ case 'i': p->up.information=1; p->up.informationset=1; break; /* Read the non-option arguments: */ case ARGP_KEY_ARG: /* Table gets only one input argument. */ if(p->up.inputset) argp_error(state, "only one input file should be given"); /* This is the first (and must be only) argument. */ p->up.inputset=1; /* See what type of input this is, and save the value. */ if( gal_fits_name_is_fits(arg) ) p->up.fitsname=arg; else p->up.txtname=arg; break; /* The command line options and arguments are finished. */ case ARGP_KEY_END: if(p->cp.setdirconf==0 && p->cp.setusrconf==0 && p->cp.printparams==0) if(state->arg_num==0) argp_error(state, "no argument given"); break; default: return ARGP_ERR_UNKNOWN; } return 0; } /* Specify the children parsers: */ struct argp_child children[]= { {&commonargp, 0, NULL, 0}, {0, 0, 0, 0} }; /* Basic structure defining the whole argument reading process. */ static struct argp thisargp = {options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif gnuastro-0.2.33-8a3b/bin/table/ui.h0000644000175000017500000000245112757417261013560 00000000000000/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef UI_H #define UI_H void checksetfge(char *optarg, int *fge, char *filename, size_t lineno); void checksetfitstabletype(char *optarg, int *fitstabletype, char *filename, size_t lineno); void setparams(int argc, char *argv[], struct tableparams *p); void freeandreport(struct tableparams *p); #endif gnuastro-0.2.33-8a3b/bin/table/ui.c0000644000175000017500000007441413004133532013541 00000000000000/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include /* From Gnulib. */ #include /* Includes time.h and sys/time.h */ #include #include #include #include "main.h" #include "ui.h" /* Needs main.h */ #include "args.h" /* Needs main.h, includes argp.h. */ /* Set the file names of the places where the default parameters are put. */ #define CONFIG_FILE SPACK CONF_POSTFIX #define SYSCONFIG_FILE SYSCONFIG_DIR "/" CONFIG_FILE #define USERCONFIG_FILEEND USERCONFIG_DIR CONFIG_FILE #define CURDIRCONFIG_FILE CURDIRCONFIG_DIR CONFIG_FILE /**************************************************************/ /************** Options and parameters ***************/ /**************************************************************/ /* Check the value given for the fge option. */ void checksetfge(char *optarg, int *fge, char *filename, size_t lineno) { *fge=optarg[0]; if( *fge!='f' && *fge!='g' && *fge!='g' ) { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, "the value of `fge' must only be one of the three " "`f', `g', or `e' characters. You have given `%s'", optarg); else error(EXIT_FAILURE, 0, "the value of `--fge' (`-f') must only be " "one of the three `f', `g', or `e' characters. You have " "given `%s'", optarg); } } void checksetfitstabletype(char *optarg, int *fitstabletype, char *filename, size_t lineno) { if( !strcmp(optarg, "ascii") ) *fitstabletype=ASCII_TBL; else if( !strcmp(optarg, "binary") ) *fitstabletype=BINARY_TBL; else { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, "The value to the `fitstabletype' must be either " "`ascii', or `binary'. You have given `%s'", optarg); else error(EXIT_FAILURE, 0, "The value to the `--fitstabletype' (`-t') " "option must be either one of `ascii', or `binary'. You have, " "given `%s'", optarg); } } void readconfig(char *filename, struct tableparams *p) { FILE *fp; size_t lineno=0, len=200; /*struct uiparams *up=&p->up;*/ struct gal_commonparams *cp=&p->cp; char *line, *name, *value, *tstring; char key='a'; /* Not used, just a place holder. */ /* When the file doesn't exist or can't be opened, it is ignored. It might be intentional, so there is no error. If a parameter is missing, it will be reported after all defaults are read. */ fp=fopen(filename, "r"); if (fp==NULL) return; /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); /* Read the tokens in the file: */ while(getline(&line, &len, fp) != -1) { /* Prepare the "name" and "value" strings, also set lineno. */ GAL_CONFIGFILES_START_READING_LINE; /* Inputs: */ if(strcmp(name, "hdu")==0) gal_checkset_allocate_copy_set(value, &cp->hdu, &cp->hduset); else if(strcmp(name, "column")==0) { gal_checkset_allocate_copy(value, &tstring); gal_linkedlist_add_to_stll(&p->up.columns, tstring); } else if(strcmp(name, "ignorecase")==0) { if(p->up.ignorecaseset) continue; gal_checkset_int_zero_or_one(value, &p->up.ignorecase, "ignorecase", key, SPACK, filename, lineno); p->up.ignorecaseset=1; } /* Outputs */ else if(strcmp(name, "output")==0) gal_checkset_allocate_copy_set(value, &cp->output, &cp->outputset); else if (strcmp(name, "feg")==0) { if(p->up.fegset) continue; checksetfge(value, &p->up.feg, filename, lineno); p->up.fegset=1; } else if (strcmp(name, "sintwidth")==0) { if(p->up.sintwidthset) continue; gal_checkset_sizet_el_zero(value, &p->up.sintwidth, name, key, SPACK, filename, lineno); p->up.sintwidthset=1; } else if (strcmp(name, "lintwidth")==0) { if(p->up.lintwidthset) continue; gal_checkset_sizet_el_zero(value, &p->up.lintwidth, name, key, SPACK, filename, lineno); p->up.lintwidthset=1; } else if (strcmp(name, "floatwidth")==0) { if(p->up.floatwidthset) continue; gal_checkset_sizet_el_zero(value, &p->up.floatwidth, name, key, SPACK, filename, lineno); p->up.floatwidthset=1; } else if (strcmp(name, "doublewidth")==0) { if(p->up.doublewidthset) continue; gal_checkset_sizet_el_zero(value, &p->up.doublewidth, name, key, SPACK, filename, lineno); p->up.doublewidthset=1; } else if (strcmp(name, "strwidth")==0) { if(p->up.strwidthset) continue; gal_checkset_sizet_el_zero(value, &p->up.strwidth, name, key, SPACK, filename, lineno); p->up.strwidthset=1; } else if (strcmp(name, "floatprecision")==0) { if(p->up.floatprecisionset) continue; gal_checkset_sizet_el_zero(value, &p->up.floatprecision, name, key, SPACK, filename, lineno); p->up.floatprecisionset=1; } else if (strcmp(name, "doubleprecision")==0) { if(p->up.doubleprecisionset) continue; gal_checkset_sizet_el_zero(value, &p->up.doubleprecision, name, key, SPACK, filename, lineno); p->up.doubleprecisionset=1; } else if (strcmp(name, "fitstabletype")==0) { if(p->up.fitstabletypeset) continue; checksetfitstabletype(value, &p->fitstabletype, filename, lineno); p->up.fitstabletypeset=1; } /* Operating modes: */ else if (strcmp(name, "information")==0) { if(p->up.informationset) continue; gal_checkset_int_zero_or_one(value, &p->up.information, name, key, SPACK, filename, lineno); p->up.informationset=1; } /* Read options common to all programs */ GAL_CONFIGFILES_READ_COMMONOPTIONS_FROM_CONF else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s` not recognized.\n", name); } free(line); fclose(fp); } void printvalues(FILE *fp, struct tableparams *p) { struct uiparams *up=&p->up; struct gal_linkedlist_stll *tmp; struct gal_commonparams *cp=&p->cp; /* Print all the options that are set. Separate each group with a commented line explaining the options in that group. */ fprintf(fp, "\n# Input:\n"); if(cp->hduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("hdu", cp->hdu); if(up->columns) for(tmp=up->columns;tmp!=NULL;tmp=tmp->next) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("column", tmp->v); if(up->ignorecaseset) fprintf(fp, CONF_SHOWFMT"%d\n", "ignorecase", up->ignorecase); fprintf(fp, "\n# Output:\n"); if(up->fegset) fprintf(fp, CONF_SHOWFMT"%c\n", "feg", up->feg); if(up->sintwidthset) fprintf(fp, CONF_SHOWFMT"%zu\n", "sintwidth", up->sintwidth); if(up->lintwidthset) fprintf(fp, CONF_SHOWFMT"%zu\n", "lintwidth", up->lintwidth); if(up->floatwidthset) fprintf(fp, CONF_SHOWFMT"%zu\n", "floatwidth", up->floatwidth); if(up->doublewidthset) fprintf(fp, CONF_SHOWFMT"%zu\n", "doublewidth", up->doublewidth); if(up->strwidthset) fprintf(fp, CONF_SHOWFMT"%zu\n", "strwidth", up->strwidth); if(up->floatprecisionset) fprintf(fp, CONF_SHOWFMT"%zu\n", "floatprecision", up->floatprecision); if(up->doubleprecisionset) fprintf(fp, CONF_SHOWFMT"%zu\n", "doubleprecision", up->doubleprecision); if(up->fitstabletypeset) fprintf(fp, CONF_SHOWFMT"%s\n", "fitstabletype", p->fitstabletype==ASCII_TBL ? "ascii" : "binary"); /* For the operating mode, first put the macro to print the common options, then the (possible options particular to this program). */ fprintf(fp, "\n# Operating mode:\n"); if(up->informationset) fprintf(fp, CONF_SHOWFMT"%d\n", "information", up->information); GAL_CONFIGFILES_PRINT_COMMONOPTIONS; } /* Note that numthreads will be used automatically based on the configure time. */ void checkifset(struct tableparams *p) { /*struct uiparams *up=&p->up;*/ struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; int intro=0; if(cp->hduset==0) GAL_CONFIGFILES_REPORT_NOTSET("hdu"); if(up->fegset==0) GAL_CONFIGFILES_REPORT_NOTSET("feg"); if(up->sintwidthset==0) GAL_CONFIGFILES_REPORT_NOTSET("sintwidth"); if(up->lintwidthset==0) GAL_CONFIGFILES_REPORT_NOTSET("lintwidth"); if(up->floatwidthset==0) GAL_CONFIGFILES_REPORT_NOTSET("floatwidth"); if(up->doublewidthset==0) GAL_CONFIGFILES_REPORT_NOTSET("doublewidth"); if(up->strwidthset==0) GAL_CONFIGFILES_REPORT_NOTSET("strwidth"); if(up->floatprecisionset==0) GAL_CONFIGFILES_REPORT_NOTSET("floatprecision"); if(up->doubleprecisionset==0) GAL_CONFIGFILES_REPORT_NOTSET("doubleprecision"); if(up->fitstabletypeset==0) GAL_CONFIGFILES_REPORT_NOTSET("fitstabletype"); GAL_CONFIGFILES_END_OF_NOTSET_REPORT; } /**************************************************************/ /************ Read and Write column info ***************/ /**************************************************************/ /* */ /* Allocate the arrays to keep the column information. Initialize the arrays with a NULL pointer to make sure that they are all found in the end if they are necessary. The values that are directly read from the input file are initialized to NULL, so they can be treated appropriately if they do not exist in the input (for example if they are mandatory, or if they need to be printed).*/ void allocinputcolinfo(struct tableparams *p) { char **c, **fc; size_t ncols=p->up.ncols; struct uiparams *up=&p->up; /* up->datatype keeps the type of data in each column as CFITSIO type macros. */ errno=0; up->datatype=malloc(ncols * sizeof *up->datatype); if(up->datatype==NULL) error(EXIT_FAILURE, errno, "%zu bytes for up->datatype", ncols * sizeof *up->datatype); /* up->ttstr keeps the actual string used to specify the datatype. */ errno=0; up->ttstr=malloc(ncols * sizeof *up->ttstr); if(up->ttstr==NULL) error(EXIT_FAILURE, errno, "%zu bytes for ttstr", ncols * sizeof *up->ttstr); fc=(c=up->ttstr)+ncols; do *c++=NULL; while(ctname keeps the name of the column. */ errno=0; up->tname=malloc(ncols * sizeof *up->tname); if(up->tname==NULL) error(EXIT_FAILURE, errno, "%zu bytes for tname", ncols * sizeof *up->tname); fc=(c=up->tname)+ncols; do *c++=NULL; while(ctunit keeps the input units of the column. */ errno=0; up->tunit=malloc(ncols * sizeof *up->tunit); if(up->tunit==NULL) error(EXIT_FAILURE, errno, "%zu bytes for tunit", ncols * sizeof *up->tunit); fc=(c=up->tunit)+ncols; do *c++=NULL; while(cup; size_t index, ncols=p->up.ncols; char keyname[FLEN_KEYWORD]="XXXXXXXXXXXXX", value[FLEN_VALUE]; /* First allocate the arrays to keep the input column information. */ allocinputcolinfo(p); /* Read all the keywords one by one and if they match, then put them in the correct value. Note that we are starting from keyword 9 because according to the FITS standard, the first 8 keys in a FITS table are reserved. */ for(i=9; strcmp(keyname, "END"); ++i) { /* Read the next keyword. */ fits_read_keyn(p->fitsptr, i, keyname, value, NULL, &status); /* Check the type of the keyword. */ if(strncmp(keyname, "TFORM", 5)==0) { /* Currently we can only read repeat==1 cases. When no number exists before the defined capital letter, it defaults to 1, but if a number exists (for example `5D'), then the repeat is 5 (there are actually five values here. Note that value[0] is a single quote.*/ if(isdigit(value[1] && value[1]!='1')) error(EXIT_FAILURE, 0, "The repeat value of column %d is " "%c, currently Table can only use columns with a repeat " "of 1.", i+1, value[1]); /* The values to TFORM are only a single character, so start the pointer to copy at 1 and put the string terminator at 3. */ value[2]='\0'; index=strtoul(&keyname[5], &tailptr, 10)-1; if(indexttstr[index] ); up->datatype[index]=gal_fits_tform_to_datatype(value[1]); } } else if(strncmp(keyname, "TTYPE", 5)==0) { /* All strings in CFITSIO start and finish with single quotation marks, CFITSIO puts them in itsself, so if we don't remove them here, we might have duplicates later, its easier to just remove them to have a simple string that might be used else where too (without the single quotes). */ value[strlen(value)-1]='\0'; index=strtoul(&keyname[5], &tailptr, 10)-1; if(indextname[index] ); } else if(strncmp(keyname, "TUNIT", 5)==0) { /* similar to tname, see above.*/ value[strlen(value)-1]='\0'; index=strtoul(&keyname[5], &tailptr, 10)-1; if(indextunit[index] ); } } /* Check if the mandatory TFORMn values are set: */ for(i=0;ittstr[i]) error(EXIT_FAILURE, 0, "TFORM%d could not be found in header", i+1); } /* Prepare column information from a text input file. Note that we are currently using Gnuastro's very simple txtarray library, which was only designed for a 2D array of floating point numbers. Later, we must update it to be more aware of the types of input columns and also accept non-number columns.*/ void alltxtcolinfo(struct tableparams *p) { size_t i; size_t ncols=p->up.ncols; /* Check if there were any strings in the array. If there were strings, then warn the user that we currently can't deal with them. */ if(gal_checkset_check_file_report(GAL_TXTARRAY_LOG)) error(EXIT_FAILURE, 0, "The input text file `%s' contained " "non-numerical values (probably strings). Please see `%s' for " "a listing of all such terms. Currently Table cannot operate on " "such files. We are working on correcting this issue.", p->up.txtname, GAL_TXTARRAY_LOG); /* Allocate the arrays to keep the input column information. */ allocinputcolinfo(p); /* Set all the column types to double and leave the other fields blank.*/ for(i=0;iup.datatype[i]=TDOUBLE; gal_checkset_allocate_copy("D", &p->up.ttstr[i] ); gal_checkset_allocate_copy("", &p->up.tname[i] ); gal_checkset_allocate_copy("", &p->up.tunit[i] ); } } /* Print the column information. */ void printinfo(struct tableparams *p) { size_t i; char *typestring=NULL; struct uiparams *up=&p->up; printf("---------------------------------------------------------\n"); if(up->fitsname) printf("%s (hdu: %s)\n", p->up.fitsname, p->cp.hdu); else printf("%s\n", p->up.txtname); printf("%-5s%-25s%-15s%s\n", "No.", "Column name", "Units", "Data type"); printf("---------------------------------------------------------\n"); for(i=0;incols;++i) { switch(up->datatype[i]) { case TBIT: typestring="bit"; break; case TBYTE: typestring="byte"; break; case TLOGICAL: typestring="logicals"; break; case TSTRING: typestring="string"; break; case TSHORT: typestring="short"; break; case TLONG: typestring="long"; break; case TLONGLONG: typestring="longlong"; break; case TFLOAT: typestring="float"; break; case TDOUBLE: typestring="double"; break; case TCOMPLEX: typestring="complex"; break; case TDBLCOMPLEX: typestring="dblcomplex"; break; case TSBYTE: typestring="signed byte"; break; case TUINT: typestring="unsigned int"; break; case TUSHORT: typestring="unsigned short"; break; default: error(EXIT_FAILURE, 0, "%d (from TFORM%zu='%c') is not a " "recognized CFITSIO datatype.", up->datatype[i], i, up->ttstr[i][0]); } printf("%-5zu%-25s%-15s%s\n", i+1, up->tname[i] ? up->tname[i] : "---", up->tunit[i] ? up->tunit[i] : "---", typestring); } /* Print the number of rows: */ printf("---------------------------------------------------------\n"); printf("Number of rows: %zu\n", p->nrows); } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ void sanitycheck(struct tableparams *p) { struct uiparams *up=&p->up; /* If the desired FITS output type is ASCII, then inform the user that this type is not yet supported. */ if(up->fitsname && p->fitstabletype==ASCII_TBL) error(EXIT_FAILURE, 0, "output to ASCII type FITS tables is currently " "not supported (due to lack of need!). If you need this feature, " "please get in touch with us at %s so we can increase the " "priority of this feature.", PACKAGE_BUGREPORT); if(up->fitsname) { /* Set the FITS pointer and check the type of the fits file. */ gal_fits_read_hdu(p->up.fitsname, p->cp.hdu, 1, &p->fitsptr); gal_fits_table_size(p->fitsptr, &p->nrows, &up->ncols); up->infitstabletype=gal_fits_table_type(p->fitsptr); allfitscolinfo(p); } else { /* Read the text file into an input array and make the basic column information. */ gal_txtarray_txt_to_array(up->txtname, &up->txtarray, &p->nrows, &up->ncols); alltxtcolinfo(p); } /* Print the column information and exit successfully if the `--information' option is given. */ if(p->up.information) { printinfo(p); freeandreport(p); exit(EXIT_SUCCESS); } /* Check the status of the output file. If no output file is set, then the output will be printed to standard output on the terminal.*/ p->outputtofits=p->outputtotxt=p->outputtostdout=0; if(p->cp.outputset) { /* First check if the file exists and remove it if it does. */ gal_checkset_check_remove_file(p->cp.output, p->cp.dontdelete); /* Now set the type of output. */ if(gal_fits_name_is_fits(p->cp.output)) p->outputtofits=1; else p->outputtotxt=1; } else p->outputtostdout=1; } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ /* FUnction to print regular expression error. This is taken from the GNU C library manual, with small modifications to fit out style, */ void regexerrorexit(int errcode, regex_t *compiled, char *input) { char *regexerrbuf; size_t length = regerror (errcode, compiled, NULL, 0); errno=0; regexerrbuf=malloc(length); if(regexerrbuf==NULL) error(EXIT_FAILURE, errno, "%zu bytes for regexerrbuf", length); (void) regerror(errcode, compiled, regexerrbuf, length); error(EXIT_FAILURE, 0, "Regular expression error: %s in value to " "`--column' (`-c'): `%s'", regexerrbuf, input); } /* If values were given to the columns option, use them to make a list of columns that must be output. Note that because regular expressions are also allowed as values to the column option, we have no idea how many columns must be printed at first, so we define a linked list to keep the column numbers for later.*/ void outputcolumns(struct tableparams *p) { long tlong; regex_t *regex; int regreturn=0; size_t i, inindex; char *tailptr, *colstring; struct uiparams *up=&p->up; struct gal_linkedlist_sll *colsll=NULL; /* Go through each given column string and take the appropriate step. */ while(p->up.columns) { /* Pop out the top node in the string linked list. */ gal_linkedlist_pop_from_stll(&p->up.columns, &colstring); /* First, see if this given column is an integer or a name/regex. If the string is an integer, then tailptr shoult point to the null character. If it points to anything else, it shows that we are not dealing with an integer (usable as a column number). So floating point values are also not acceptable. */ tlong=strtol(colstring, &tailptr,0); if(*tailptr=='\0') { /* Make sure we are not dealing with a negative number! */ if(tlong<0) error(EXIT_FAILURE, 0, "the column numbers given to the " "`--column' (`-c') option must not be negative, you " "have given a value of `%ld'", tlong); /* Check if the given value is not larger than the number of columns in the input catalog. */ if(tlong>up->ncols) error(EXIT_FAILURE, 0, "%s (hdu: %s) has %zu columns, but " "you have asked for column number %zu", p->up.fitsname, p->cp.hdu, up->ncols, tlong); /* Everything seems to be fine, put this column number in the output column numbers linked list. Note that internally, the column numbers start from 0, not 1.*/ gal_linkedlist_add_to_sll(&colsll, tlong-1); } else { /* Allocate the regex_t structure: */ errno=0; regex=malloc(sizeof *regex); if(regex==NULL) error(EXIT_FAILURE, errno, "%zu bytes for regex", sizeof *regex); /* Go through all the columns names and see if this matches them. But first we have to "compile" the string into the regular expression, see the "POSIX Regular Expression Compilation" section of the GNU C Library. About the case of the string: the FITS standard says: "It is _strongly recommended_ that every field of the table be assigned a unique, case insensitive name with this keyword..." So the column names can be case-sensitive. Here, we don't care about the details of a match, the only important thing is a match, so we are using the REG_NOSUB flag.*/ regreturn=0; regreturn=regcomp(regex, colstring, ( p->up.ignorecase ? REG_NOSUB + REG_ICASE : REG_NOSUB ) ); if(regreturn) regexerrorexit(regreturn, regex, colstring); /* With the regex structure "compile"d you can go through all the column names. Just note that column names are not mandatory in the FITS standard, so some (or all) columns might not have names, if so `p->tname[i]' will be NULL. */ for(i=0;incols;++i) if(up->tname[i] && regexec(regex, up->tname[i], 0, 0, 0)==0) gal_linkedlist_add_to_sll(&colsll, i); /* Free the regex_t structure: */ regfree(regex); } /* We don't need this user provided column string any more. */ free(colstring); } /* Based on the number of columns found above, allocate an array of `outcolumn' structures to keep the information for each column. */ p->nocols=gal_linkedlist_num_in_sll(colsll); errno=0; p->ocols=malloc(p->nocols*sizeof *p->ocols); if(p->ocols==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->ocols", p->nocols*sizeof *p->ocols); /* Fill in the output column with the needed input table information. Note that a simple linked list is first-in-last-out, so we have to fill in the output columns in reverse order. Also, note that we are popping from the linked list keeping the indexs of the output columns and thus also freeing their allocated space. */ i=p->nocols-1; while(colsll) { gal_linkedlist_pop_from_sll(&colsll, &inindex); p->ocols[i].inindex=inindex; p->ocols[i].datatype=up->datatype[inindex]; p->ocols[i].esize=gal_fits_datatype_size(up->datatype[inindex]); --i; } } void preparearrays(struct tableparams *p) { size_t i; struct uiparams *up=&p->up; /* Reverse the columns linked list here (before possibly printing).*/ gal_linkedlist_reverse_stll(&up->columns); /* Set the columns that should be included in the output. If up->columns is set, then use it, otherwise, set all the columns for printing. */ if(p->up.columns) outputcolumns(p); else { p->nocols=up->ncols; errno=0; p->ocols=malloc(p->nocols * sizeof *p->ocols); if(p->ocols==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->ocols", p->nocols * sizeof *p->ocols); for(i=0;inocols;++i) { p->ocols[i].inindex=i; p->ocols[i].datatype=up->datatype[i]; p->ocols[i].esize=gal_fits_datatype_size(p->ocols[i].datatype); } } } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void setparams(int argc, char *argv[], struct tableparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; /* Set the non-zero initial values, the structure was initialized to have a zero value for all elements. */ cp->spack = SPACK; cp->verb = 1; cp->numthreads = num_processors(NPROC_CURRENT); cp->removedirinfo = 1; /* Initialize this utility's pointers to NULL. */ p->ocols=NULL; up->columns=NULL; up->txtname=up->fitsname=NULL; up->ttstr=up->tname=up->tunit=NULL; /* Read the arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Add the user default values and save them if asked. */ GAL_CONFIGFILES_CHECK_SET_CONFIG; /* Check if all the required parameters are set. */ checkifset(p); /* Print the values for each parameter. */ if(cp->printparams) GAL_CONFIGFILES_REPORT_PARAMETERS_SET; /* Do a sanity check. */ sanitycheck(p); /* Make the array of input images. */ preparearrays(p); } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void freeandreport(struct tableparams *p) { size_t i, j; int status=0; char **rowofstrings; struct uiparams *up=&p->up; /* Free the allocated arrays: */ free(p->cp.hdu); free(up->txtarray); free(up->datatype); free(p->cp.output); /* Free the input column information: */ for(i=0;incols;++i) { if(up->ttstr) free(up->ttstr[i]); if(up->tname) free(up->tname[i]); if(up->tunit) free(up->tunit[i]); } free(up->ttstr); free(up->tname); free(up->tunit); /* Free the output column information: */ for(i=0;inocols;++i) { free(p->ocols[i].nulval); if(p->ocols[i].datatype==TSTRING) { rowofstrings=(char **)(p->ocols[i].data); for(j=0;jnrows;++j) free(rowofstrings[j]); } else free(p->ocols[i].data); } free(p->ocols); /* Close the FITS file: */ if(p->up.fitsname && fits_close_file(p->fitsptr, &status)) gal_fits_io_error(status, NULL); } gnuastro-0.2.33-8a3b/bin/table/cite.h0000644000175000017500000000316312757417261014070 00000000000000/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CITE_H #define CITE_H #define TABLEBIBTEX "" #define PRINTCITEABORT { \ printf("\nWe hope %s has been useful for your research.\n" \ "Citations are vital for the continued work on %s.\n" \ "Thank you for citing it in your research paper.\n" \ "\nPlease cite as \"%s\":\n\n%s\n\n%s", \ SPACK_NAME, SPACK_NAME, SPACK_STRING, \ GAL_STRINGS_MAIN_BIBTEX, TABLEBIBTEX); \ exit(EXIT_SUCCESS); \ } #endif gnuastro-0.2.33-8a3b/bin/table/main.h0000644000175000017500000001153313002500335014043 00000000000000/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include #include /* Progarm name macros: */ #define SPACK "asttable" /* Subpackage executable name. */ #define SPACK_NAME "Table" /* Subpackage full name. */ #define SPACK_STRING SPACK_NAME" ("PACKAGE_NAME") "PACKAGE_VERSION #define MAX_COL_FORMAT_LENGTH 20 /* Structure to keep the information for each output column */ struct outcolumn { size_t inindex; /* Row index (from 0) in input array. */ int datatype; /* Type of data (from CFITSIO macros). */ int anynul; /* If there is any blank characters. */ void *nulval; /* The blank value for this column. */ void *data; /* Array keeping the column data. */ size_t esize; /* Size of each element in this column. */ char fmt[MAX_COL_FORMAT_LENGTH]; /* format to use in printf. */ }; /* User interface structure. */ struct uiparams { int information; /* ==1, only print FITS information. */ char *fitsname; /* Name of input FITS file. */ char *txtname; /* Name of input text file. */ int ignorecase; /* Ignore case matching column names. */ /* Input table parameters. */ size_t ncols; /* Number of columns in table. */ int *datatype; /* Type of data in column. */ char **ttstr; /* TFORM (another format for type). */ char **tname; /* Column name (one word). */ char **tunit; /* Unit of values in column. */ double *txtarray; /* Array keeping text file values. */ int infitstabletype; /* Input table is ASCII or binary. */ /* Print parameters: */ int feg; /* format of floating points. */ size_t sintwidth; /* Full width for short integers. */ size_t lintwidth; /* Full width for short integers. */ size_t floatwidth; /* Full width for all floats. */ size_t doublewidth; /* Full width for all doubles. */ size_t strwidth; /* Full width for all floats. */ size_t floatprecision; /* Number of decimals for floats. */ size_t doubleprecision; /* Number of decimals for doubles. */ /* If values are set: */ int inputset; int informationset; int ignorecaseset; int fegset; int sintwidthset; int lintwidthset; int floatwidthset; int doublewidthset; int strwidthset; int floatprecisionset; int doubleprecisionset; int fitstabletypeset; struct gal_linkedlist_stll *columns; }; /* Main program parameters structure */ struct tableparams { /* Other structures: */ struct uiparams up; /* User interface parameters. */ struct gal_commonparams cp; /* Common parameters. */ /* Input: */ fitsfile *fitsptr; /* FITS pointer (input or output). */ /* Output: */ size_t nrows; /* Number of rows in table. */ size_t nocols; /* Number of output columns. */ struct outcolumn *ocols; /* Array of output column informatio. */ int outputtofits; /* ==1: output is a FITS file. */ int outputtotxt; /* ==1: output is a text file. */ int outputtostdout; /* ==1: output is the standard output. */ int fitstabletype; /* ASCII, or binary table CFITSIO macro.*/ /* Internal: */ int onlyview; time_t rawtime; /* Starting time of the program. */ }; #endif gnuastro-0.2.33-8a3b/bin/table/main.c0000644000175000017500000000313412774160341014052 00000000000000/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include /* Includes time.h and sys/time.h */ #include "main.h" #include "ui.h" /* needs main.h. */ #include "table.h" /* needs main.h. */ int main (int argc, char *argv[]) { struct tableparams p={{0}, {0}, 0}; /* Set they starting time. */ time(&p.rawtime); /* Read the input parameters. */ setparams(argc, argv, &p); /* Run MakeProfiles */ table(&p); /* Free all non-freed allocations. */ freeandreport(&p); /* Return successfully.*/ return EXIT_SUCCESS; } gnuastro-0.2.33-8a3b/bin/table/Makefile.in0000644000175000017500000017245213004464627015042 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is 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GNULIB_BTOWC = @GNULIB_BTOWC@ GNULIB_CALLOC_POSIX = @GNULIB_CALLOC_POSIX@ GNULIB_CANONICALIZE_FILE_NAME = @GNULIB_CANONICALIZE_FILE_NAME@ GNULIB_CBRT = @GNULIB_CBRT@ GNULIB_CBRTF = @GNULIB_CBRTF@ GNULIB_CBRTL = @GNULIB_CBRTL@ GNULIB_CEIL = @GNULIB_CEIL@ GNULIB_CEILF = @GNULIB_CEILF@ GNULIB_CEILL = @GNULIB_CEILL@ GNULIB_CHDIR = @GNULIB_CHDIR@ GNULIB_CHOWN = @GNULIB_CHOWN@ GNULIB_CLOSE = @GNULIB_CLOSE@ GNULIB_COPYSIGN = @GNULIB_COPYSIGN@ GNULIB_COPYSIGNF = @GNULIB_COPYSIGNF@ GNULIB_COPYSIGNL = @GNULIB_COPYSIGNL@ GNULIB_COSF = @GNULIB_COSF@ GNULIB_COSHF = @GNULIB_COSHF@ GNULIB_COSL = @GNULIB_COSL@ GNULIB_DPRINTF = @GNULIB_DPRINTF@ GNULIB_DUP = @GNULIB_DUP@ GNULIB_DUP2 = @GNULIB_DUP2@ GNULIB_DUP3 = @GNULIB_DUP3@ GNULIB_DUPLOCALE = @GNULIB_DUPLOCALE@ GNULIB_ENVIRON = @GNULIB_ENVIRON@ GNULIB_EUIDACCESS = @GNULIB_EUIDACCESS@ GNULIB_EXP2 = @GNULIB_EXP2@ GNULIB_EXP2F = @GNULIB_EXP2F@ GNULIB_EXP2L = @GNULIB_EXP2L@ GNULIB_EXPF = @GNULIB_EXPF@ GNULIB_EXPL = @GNULIB_EXPL@ GNULIB_EXPM1 = @GNULIB_EXPM1@ GNULIB_EXPM1F = @GNULIB_EXPM1F@ GNULIB_EXPM1L = @GNULIB_EXPM1L@ GNULIB_FABSF = @GNULIB_FABSF@ GNULIB_FABSL = @GNULIB_FABSL@ GNULIB_FACCESSAT = @GNULIB_FACCESSAT@ GNULIB_FCHDIR = @GNULIB_FCHDIR@ GNULIB_FCHMODAT = @GNULIB_FCHMODAT@ GNULIB_FCHOWNAT = @GNULIB_FCHOWNAT@ GNULIB_FCLOSE = @GNULIB_FCLOSE@ GNULIB_FCNTL = @GNULIB_FCNTL@ GNULIB_FDATASYNC = @GNULIB_FDATASYNC@ GNULIB_FDOPEN = @GNULIB_FDOPEN@ GNULIB_FFLUSH = @GNULIB_FFLUSH@ GNULIB_FFS = @GNULIB_FFS@ GNULIB_FFSL = @GNULIB_FFSL@ GNULIB_FFSLL = @GNULIB_FFSLL@ GNULIB_FGETC = @GNULIB_FGETC@ GNULIB_FGETS = @GNULIB_FGETS@ GNULIB_FLOOR = @GNULIB_FLOOR@ GNULIB_FLOORF = @GNULIB_FLOORF@ GNULIB_FLOORL = @GNULIB_FLOORL@ GNULIB_FMA = @GNULIB_FMA@ GNULIB_FMAF = @GNULIB_FMAF@ GNULIB_FMAL = @GNULIB_FMAL@ GNULIB_FMOD = @GNULIB_FMOD@ GNULIB_FMODF = @GNULIB_FMODF@ GNULIB_FMODL = @GNULIB_FMODL@ GNULIB_FOPEN = @GNULIB_FOPEN@ GNULIB_FPRINTF = @GNULIB_FPRINTF@ GNULIB_FPRINTF_POSIX = @GNULIB_FPRINTF_POSIX@ GNULIB_FPURGE = @GNULIB_FPURGE@ GNULIB_FPUTC = @GNULIB_FPUTC@ GNULIB_FPUTS = @GNULIB_FPUTS@ GNULIB_FREAD = @GNULIB_FREAD@ GNULIB_FREOPEN = @GNULIB_FREOPEN@ GNULIB_FREXP = @GNULIB_FREXP@ GNULIB_FREXPF = @GNULIB_FREXPF@ GNULIB_FREXPL = @GNULIB_FREXPL@ GNULIB_FSCANF = @GNULIB_FSCANF@ GNULIB_FSEEK = @GNULIB_FSEEK@ GNULIB_FSEEKO = @GNULIB_FSEEKO@ GNULIB_FSTAT = @GNULIB_FSTAT@ GNULIB_FSTATAT = @GNULIB_FSTATAT@ GNULIB_FSYNC = @GNULIB_FSYNC@ GNULIB_FTELL = @GNULIB_FTELL@ GNULIB_FTELLO = @GNULIB_FTELLO@ GNULIB_FTRUNCATE = @GNULIB_FTRUNCATE@ GNULIB_FUTIMENS = @GNULIB_FUTIMENS@ GNULIB_FWRITE = @GNULIB_FWRITE@ GNULIB_GETC = @GNULIB_GETC@ GNULIB_GETCHAR = @GNULIB_GETCHAR@ GNULIB_GETCWD = @GNULIB_GETCWD@ GNULIB_GETDELIM = @GNULIB_GETDELIM@ GNULIB_GETDOMAINNAME = @GNULIB_GETDOMAINNAME@ GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = 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.NOEXPORT: gnuastro-0.2.33-8a3b/bin/table/asttable.conf0000644000175000017500000000163212757417261015440 00000000000000# Default parameters (System) for Table. # Table is part of GNU Astronomy Utitlies. # # Use the long option name of each paramter followed by # a value. The name and value should be separated by # atleast one of the following charaacters: # space, `,`, `=` or `:` # # Run with `--help` option or read the manual for a full # explanation of what each option means. # # NOTE I: All counting is from zero, not one. # NOTE II: Lines starting with `#` are ignored. # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Input: hdu 0 # Output: feg f sintwidth 5 lintwidth 15 floatwidth 10 doublewidth 15 strwidth 20 floatprecision 3 doubleprecision 8 fitstabletype binary gnuastro-0.2.33-8a3b/bin/table/Makefile.am0000644000175000017500000000267712765246727015046 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2016, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. NOTE: $(top_srcdir)/bootstrapped/lib is only necessary ## for internally compiled utilities and libraries. It must not be included ## during the tests since the bootstrapped libraries are not installed. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Utility and its sources bin_PROGRAMS = asttable asttable_SOURCES = main.c main.h cite.h ui.c ui.h args.h \ table.c table.h asttable_LDADD = $(top_builddir)/bootstrapped/lib/libgnu.la \ -lgnuastro ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = asttable.conf gnuastro-0.2.33-8a3b/bin/subtractsky/0000755000175000017500000000000013004464725014330 500000000000000gnuastro-0.2.33-8a3b/bin/subtractsky/subtractsky.h0000644000175000017500000000212212616616510016773 00000000000000/********************************************************************* SubtractSky - Find and subtract the sky value from an image. SubtractSky is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef SUBTRACTSKY_H #define SUBTRACTSKY_H void subtractsky(struct subtractskyparams *p); #endif gnuastro-0.2.33-8a3b/bin/subtractsky/subtractsky.c0000644000175000017500000002002413001632540016755 00000000000000/********************************************************************* SubtractSky - Find and subtract the sky value from an image. SubtractSky is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include "main.h" void * avestdonthread(void *inparam) { struct gal_mesh_thread_params *mtp=(struct gal_mesh_thread_params *)inparam; struct gal_mesh_params *mp=mtp->mp; struct subtractskyparams *p=(struct subtractskyparams *)mp->params; float *mponeforall=mp->oneforall; float *oneforall=&mponeforall[mtp->id*mp->maxs0*mp->maxs1]; float *f, *cofa, *c=NULL; /* cofa: convolved-oneforall */ size_t modeindex=(size_t)(-1); size_t s0, s1, ind, row, num, start, is1=mp->s1; size_t i, *indexs=&mp->indexs[mtp->id*mp->thrdcols]; float mirrordist=mp->mirrordist, minmodeq=mp->minmodeq; float ave, med, std, *sorted, sigclipmultip=p->sigclipmultip; float *imgend, *inimg=mp->img, *inconv=p->conv, modesym=0.0f; float *conv=NULL, *img, sigcliptolerance=p->sigcliptolerance; /* Allocate the oneforall array for the convolved image, since we only want to use those meshs whose convolved image mode is larger than minmodeq. */ if(p->conv!=mp->img) { errno=0; cofa=malloc(mp->maxs0*mp->maxs1*sizeof *oneforall); if(cofa==NULL) error(EXIT_FAILURE, errno, "unable to allocate %zu bytes for" "cofa in avestdonthread of subtractsky.c", mp->maxs0*mp->maxs1*sizeof *mp->img); } else cofa=NULL; /* Start this thread's work: */ for(i=0;indexs[i]!=GAL_THREADS_NON_THRD_INDEX;++i) { /* Prepare the values: */ num=row=0; f=oneforall; ind=indexs[i]; start=mp->start[ind]; s0=mp->ts0[mp->types[ind]]; s1=mp->ts1[mp->types[ind]]; if(cofa) c=sorted=cofa; else sorted=oneforall; /* Copy all the non-NaN pixels images pixels of this mesh into the mesh array. Note that currently, the spatial positioning of the pixels is irrelevant, so we only keep those that are non-NaN. Recall that both the convolved an unconvolved image have the same NaN pixels.*/ do { if(cofa) conv = inconv + start + row * is1; imgend=(img = inimg + start + row++ * is1 ) + s1; do { if(!isnan(*img)) { ++num; *f++ = *img; if(cofa) *c++=*conv; } if(cofa) ++conv; } while(++imgGAL_STATISTICS_MODE_SYM_GOOD && (float)modeindex/(float)num>minmodeq ) { /* If cofa was defined, then oneforall was not sorted. */ if(cofa) qsort(oneforall, num, sizeof *oneforall, gal_qsort_float_increasing); /* Do sigma-clipping and save the result if it is accurate. Note that all meshs were initialized to NaN, so if they don't fit the criteria, they can simply be ignored. */ if(gal_statistics_sigma_clip_converge(oneforall, 1, num, sigclipmultip, sigcliptolerance, &ave, &med, &std, 0)) { mp->cgarray1[ind]=ave; if(mp->ngarrays==2) mp->cgarray2[ind]=std; } } } /* Free any allocated space and if multiple threads were used, wait until all other threads finish. */ if(p->conv!=mp->img) free(cofa); if(mp->numthreads>1) pthread_barrier_wait(&mp->b); return NULL; } void subtractsky(struct subtractskyparams *p) { struct gal_mesh_params *mp=&p->mp; long *meshindexs; struct timeval t1; int checkstd=p->checkstd; size_t s0=mp->s0, s1=mp->s1; float *sky, *std, *skysubtracted; /* Prepare the mesh array. */ gettimeofday(&t1, NULL); gal_mesh_make_mesh(mp); if(p->meshname) { gal_mesh_check_mesh_id(mp, &meshindexs); gal_fits_array_to_file(p->meshname, "Input", FLOAT_IMG, p->mp.img, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); gal_fits_array_to_file(p->meshname, "MeshIndexs", LONG_IMG, meshindexs, s0, s1, 0, p->wcs, NULL, SPACK_STRING); free(meshindexs); } if(p->cp.verb) gal_timing_report(&t1, "Mesh grid ready.", 1); /* Convolve the image if the user has asked for it: */ if(p->up.kernelnameset) { gal_mesh_spatial_convolve_on_mesh(mp, &p->conv); if(p->convname) { gal_fits_array_to_file(p->convname, "Input", FLOAT_IMG, p->mp.img, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); gal_fits_array_to_file(p->convname, "Input", FLOAT_IMG, p->conv, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); } } else p->conv=p->mp.img; if(p->cp.verb) gal_timing_report(&t1, "Input image convolved with kernel.", 1); /* Find the sky value and its standard deviation on each mesh. */ gal_mesh_operate_on_mesh(mp, avestdonthread, sizeof(float), checkstd, 1); if(p->skyname) gal_mesh_value_file(mp, p->skyname, "Sky value", "Sky STD", p->wcs, SPACK_STRING); if(p->cp.verb) gal_timing_report(&t1, "Sky and its STD found on some meshes.", 1); /* Interpolate over the meshs to fill all the blank ones in both the sky and the standard deviation arrays: */ gal_mesh_interpolate(mp, "Interpolating the sky and its standard deviation"); if(p->skyname) gal_mesh_value_file(mp, p->skyname, "Sky Interpolated", "Sky STD interpolated", p->wcs, SPACK_STRING); if(p->cp.verb) gal_timing_report(&t1, "All blank meshs filled (interplated).", 1); /* Smooth the interpolated array: */ if(mp->smoothwidth>1) { gal_mesh_smooth(mp); if(p->cp.verb) gal_timing_report(&t1, "Mesh grid smoothed.", 1); } /* Make the sky array and save it if the user has asked for it: */ gal_mesh_check_garray(mp, &sky, &std); if(p->skyname) gal_mesh_value_file(mp, p->skyname, "Sky Smoothed", "Sky STD smoothed", p->wcs, SPACK_STRING); /* Subtract the sky value */ gal_array_fmultip_const(sky, s0*s1, -1.0f); skysubtracted=gal_array_fsum_arrays(mp->img, sky, s0*s1); gal_fits_array_to_file(p->cp.output ,"SkySubtracted", FLOAT_IMG, skysubtracted, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); /* Clean up: */ free(sky); gal_mesh_free_mesh(mp); free(skysubtracted); if(checkstd) free(std); if(p->up.kernelnameset) free(p->conv); } gnuastro-0.2.33-8a3b/bin/subtractsky/args.h0000644000175000017500000002426512774161241015366 00000000000000/********************************************************************* SubtractSky - Find and subtract the sky value from an image. SubtractSky is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef ARGS_H #define ARGS_H #include #include #include /**************************************************************/ /************** argp.h definitions ***************/ /**************************************************************/ /* Definition parameters for the argp: */ const char *argp_program_version=SPACK_STRING"\n"GAL_STRINGS_COPYRIGHT "\n\nWritten by Mohammad Akhlaghi"; const char *argp_program_bug_address=PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata"; const char doc[] = /* Before the list of options: */ GAL_STRINGS_TOP_HELP_INFO SPACK_NAME" Finds the sky value over a grid on the input and subtracts " "it from the image to give a clear and uniform output. \n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /* Available letters for short options: c e f g i j l m p r v w x y z A B C E F G I J O R W X Y Z Number keys free: >=510 Options with keys (second structure element) larger than 500 do not have a short version. */ static struct argp_option options[] = { { 0, 0, 0, 0, "Input:", 1 }, { "mask", 'M', "STR", 0, "Mask image file name.", 1 }, { "mhdu", 'H', "STR", 0, "Mask image header name.", 1 }, { "kernel", 'k', "STR", 0, "Kernel image file name for convolution.", 1 }, { "khdu", 'U', "STR", 0, "Kernel image header name for convolution.", 1 }, { 0, 0, 0, 0, "Output:", 2 }, { "checksky", 502, 0, 0, "Store final sky and its STD in `_sky.fits' file.", 2 }, { "checkskystd", 505, 0, 0, "Include sky standard deviation in all checks too.", 2 }, { "checkconvolution", 507, 0, 0, "Store convolved image in `_conv.fits' file.", 2 }, { 0, 0, 0, 0, "Mesh grid:", 3 }, { "meshsize", 's', "INT", 0, "Size of each mesh (tile) in the grid.", 3 }, { "nch1", 'a', "INT", 0, "Number of channels along first FITS axis.", 3 }, { "nch2", 'b', "INT", 0, "Number of channels along second FITS axis.", 3 }, { "lastmeshfrac", 'L', "INT", 0, "Fraction of last mesh area to add new.", 3 }, { "mirrordist", 'd', "FLT", 0, "Distance beyond mirror point. Multiple of std.", 3 }, { "minmodeq", 'Q', "FLT", 0, "Minimum acceptable quantile for the mode.", 3 }, { "interponlyblank", 508, 0, 0, "Only interpolate over the blank pixels.", 3 }, { "numnearest", 'n', "INT", 0, "Number of nearest neighbors to interpolate.", 3 }, { "smoothwidth", 'T', "INT", 0, "Width of smoothing kernel (odd number).", 3 }, { "fullconvolution", 506, 0, 0, "Ignore channels in imageconvolution.", 3 }, { "fullinterpolation", 503, 0, 0, "Ignore channels in interpolation.", 3 }, { "fullsmooth", 504, 0, 0, "Ignore channels in smoothing.", 3 }, { "checkmesh", 500, 0, 0, "Store mesh IDs in `_mesh.fits' file.", 3 }, { "meshbasedcheck", 501, 0, 0, "Each mesh in one pixel in mesh check images.", 3 }, { 0, 0, 0, 0, "Statistics:", 4 }, { "sigclipmultip", 'u', "FLT", 0, "Multiple of standard deviation in sigma-clipping.", 4 }, { "sigcliptolerance", 't', "FLT", 0, "Difference in STD tolerance to halt iteration.", 4 }, { 0, 0, 0, 0, "Operating modes:", -1 }, {0} }; /* Parse a single option: */ static error_t parse_opt(int key, char *arg, struct argp_state *state) { /* Save the arguments structure: */ struct subtractskyparams *p = state->input; /* Set the pointer to the common parameters for all programs here: */ state->child_inputs[0]=&p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); switch(key) { /* Input: */ case 'M': gal_checkset_allocate_copy_set(arg, &p->up.maskname, &p->up.masknameset); break; case 'H': gal_checkset_allocate_copy_set(arg, &p->up.mhdu, &p->up.mhduset); break; case 'K': gal_checkset_allocate_copy_set(arg, &p->up.kernelname, &p->up.kernelnameset); break; case 'U': gal_checkset_allocate_copy_set(arg, &p->up.khdu, &p->up.khduset); break; /* Output: */ case 502: p->skyname="a"; break; case 505: p->checkstd=1; break; /* Mesh grid: */ case 's': gal_checkset_sizet_l_zero(arg, &p->mp.meshsize, "meshsize", key, SPACK, NULL, 0); p->up.meshsizeset=1; break; case 'a': gal_checkset_sizet_l_zero(arg, &p->mp.nch1, "nch1", key, SPACK, NULL, 0); p->up.nch1set=1; break; case 'b': gal_checkset_sizet_l_zero(arg, &p->mp.nch2, "nch2", key, SPACK, NULL, 0); p->up.nch2set=1; break; case 'L': gal_checkset_float_l_0_s_1(arg, &p->mp.lastmeshfrac, "lastmeshfrac", key, SPACK, NULL, 0); p->up.lastmeshfracset=1; break; case 'd': gal_checkset_float_l_0(arg, &p->mp.mirrordist, "mirrordist", key, SPACK, NULL, 0); p->up.mirrordistset=1; break; case 'Q': gal_checkset_float_l_0_s_1(arg, &p->mp.minmodeq, "minmodeq", key, SPACK, NULL, 0); p->up.minmodeqset=1; break; case 508: p->mp.interponlyblank=1; break; case 'n': gal_checkset_sizet_l_zero(arg, &p->mp.numnearest, "numnearest", key, SPACK, NULL, 0); p->up.numnearestset=1; break; case 'T': gal_checkset_sizet_p_odd(arg, &p->mp.smoothwidth, "smoothwidth", key, SPACK, NULL, 0); p->up.smoothwidthset=1; break; case 506: p->mp.fullconvolution=1; p->up.fullconvolutionset=1; break; case 503: p->mp.fullinterpolation=1; p->up.fullinterpolationset=1; break; case 504: p->mp.fullsmooth=1; p->up.fullsmoothset=1; break; case 500: p->meshname="a"; /* Just a placeholder! It will be corrected later */ break; case 507: p->convname="a"; break; case 501: p->mp.meshbasedcheck=1; break; /* Statistics */ case 'u': gal_checkset_float_l_0(arg, &p->sigclipmultip, "sigclipmultip", key, SPACK, NULL, 0); p->up.sigclipmultipset=1; break; case 't': gal_checkset_float_l_0_s_1(arg, &p->sigcliptolerance, "sigcliptolerance", key, SPACK, NULL, 0); p->up.sigcliptoleranceset=1; break; /* Operating modes: */ /* Read the non-option arguments: */ case ARGP_KEY_ARG: /* See what type of input value it is and put it in. */ if( gal_fits_name_is_fits(arg) ) { if(p->up.inputname) argp_error(state, "only one input image should be given"); else p->up.inputname=arg; } else argp_error(state, "%s is not a valid file type", arg); break; /* The command line options and arguments are finished. */ case ARGP_KEY_END: if(p->cp.setdirconf==0 && p->cp.setusrconf==0 && p->cp.printparams==0) { if(state->arg_num==0) argp_error(state, "no argument given"); if(p->up.inputname==NULL) argp_error(state, "no input FITS image(s) provided"); } break; default: return ARGP_ERR_UNKNOWN; } return 0; } /* Specify the children parsers: */ struct argp_child children[]= { {&commonargp, 0, NULL, 0}, {0, 0, 0, 0} }; /* Basic structure defining the whole argument reading process. */ static struct argp thisargp = {options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif gnuastro-0.2.33-8a3b/bin/subtractsky/ui.h0000644000175000017500000000225012616616510015034 00000000000000/********************************************************************* SubtractSky - Find and subtract the sky value from an image. SubtractSky is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef IMCROPUI_H #define IMCROPUI_H void setparams(int argc, char *argv[], struct subtractskyparams *p); void freeandreport(struct subtractskyparams *p, struct timeval *t1); #endif gnuastro-0.2.33-8a3b/bin/subtractsky/ui.c0000644000175000017500000004400413001632540015020 00000000000000/********************************************************************* SubtractSky - Find and subtract the sky value from an image. SubtractSky is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include /* From Gnulib. */ #include /* Includes time.h and sys/time.h */ #include #include #include #include "main.h" #include "ui.h" /* Needs main.h */ #include "args.h" /* Needs main.h, includes argp.h. */ /* Set the file names of the places where the default parameters are put. */ #define CONFIG_FILE SPACK CONF_POSTFIX #define SYSCONFIG_FILE SYSCONFIG_DIR "/" CONFIG_FILE #define USERCONFIG_FILEEND USERCONFIG_DIR CONFIG_FILE #define CURDIRCONFIG_FILE CURDIRCONFIG_DIR CONFIG_FILE /**************************************************************/ /************** Options and parameters ***************/ /**************************************************************/ void readconfig(char *filename, struct subtractskyparams *p) { FILE *fp; size_t lineno=0, len=200; char *line, *name, *value; struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; char key='a'; /* Not used, just a place holder. */ /* When the file doesn't exist or can't be opened, it is ignored. It might be intentional, so there is no error. If a parameter is missing, it will be reported after all defaults are read. */ fp=fopen(filename, "r"); if (fp==NULL) return; /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); /* Read the tokens in the file: */ while(getline(&line, &len, fp) != -1) { /* Prepare the "name" and "value" strings, also set lineno. */ GAL_CONFIGFILES_START_READING_LINE; /* Inputs: */ if(strcmp(name, "hdu")==0) gal_checkset_allocate_copy_set(value, &cp->hdu, &cp->hduset); else if(strcmp(name, "mask")==0) gal_checkset_allocate_copy_set(value, &up->maskname, &up->masknameset); else if(strcmp(name, "mhdu")==0) gal_checkset_allocate_copy_set(value, &up->mhdu, &up->mhduset); else if(strcmp(name, "kernel")==0) gal_checkset_allocate_copy_set(value, &up->kernelname, &up->kernelnameset); else if(strcmp(name, "khdu")==0) gal_checkset_allocate_copy_set(value, &up->khdu, &up->khduset); /* Outputs */ else if(strcmp(name, "output")==0) gal_checkset_allocate_copy_set(value, &cp->output, &cp->outputset); /* Mesh grid: */ else if(strcmp(name, "meshsize")==0) { if(up->meshsizeset) continue; gal_checkset_sizet_l_zero(value, &p->mp.meshsize, name, key, SPACK, filename, lineno); up->meshsizeset=1; } else if(strcmp(name, "nch1")==0) { if(up->nch1set) continue; gal_checkset_sizet_l_zero(value, &p->mp.nch1, name, key, SPACK, filename, lineno); up->nch1set=1; } else if(strcmp(name, "nch2")==0) { if(up->nch2set) continue; gal_checkset_sizet_l_zero(value, &p->mp.nch2, name, key, SPACK, filename, lineno); up->nch2set=1; } else if(strcmp(name, "lastmeshfrac")==0) { if(up->lastmeshfracset) continue; gal_checkset_float_l_0_s_1(value, &p->mp.lastmeshfrac, name, key, SPACK, filename, lineno); up->lastmeshfracset=1; } else if(strcmp(name, "mirrordist")==0) { if(up->mirrordistset) continue; gal_checkset_float_l_0(value, &p->mp.mirrordist, name, key, SPACK, filename, lineno); up->mirrordistset=1; } else if(strcmp(name, "minmodeq")==0) { if(up->minmodeqset) continue; gal_checkset_float_l_0_s_1(value, &p->mp.minmodeq, name, key, SPACK, filename, lineno); up->minmodeqset=1; } else if(strcmp(name, "numnearest")==0) { if(up->numnearestset) continue; gal_checkset_sizet_l_zero(value, &p->mp.numnearest, name, key, SPACK, filename, lineno); up->numnearestset=1; } else if(strcmp(name, "smoothwidth")==0) { if(up->smoothwidthset) continue; gal_checkset_sizet_p_odd(value, &p->mp.smoothwidth, name, key, SPACK, filename, lineno); up->smoothwidthset=1; } else if(strcmp(name, "fullconvolution")==0) { if(up->fullconvolutionset) continue; gal_checkset_int_zero_or_one(value, &p->mp.fullconvolution, name, key, SPACK, filename, lineno); up->fullconvolutionset=1; } else if(strcmp(name, "fullinterpolation")==0) { if(up->fullinterpolationset) continue; gal_checkset_int_zero_or_one(value, &p->mp.fullinterpolation, name, key, SPACK, filename, lineno); up->fullinterpolationset=1; } else if(strcmp(name, "fullsmooth")==0) { if(up->fullsmoothset) continue; gal_checkset_int_zero_or_one(value, &p->mp.fullsmooth, name, key, SPACK, filename, lineno); up->fullsmoothset=1; } /* Statistics: */ else if(strcmp(name, "sigclipmultip")==0) { if(up->sigclipmultipset) continue; gal_checkset_float_l_0(value, &p->sigclipmultip, name, key, SPACK, filename, lineno); up->sigclipmultipset=1; } else if(strcmp(name, "sigcliptolerance")==0) { if(up->sigcliptoleranceset) continue; gal_checkset_float_l_0_s_1(value, &p->sigcliptolerance, name, key, SPACK, filename, lineno); up->sigcliptoleranceset=1; } /* Operating modes: */ /* Read options common to all programs */ GAL_CONFIGFILES_READ_COMMONOPTIONS_FROM_CONF else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s` not recognized.\n", name); } free(line); fclose(fp); } void printvalues(FILE *fp, struct subtractskyparams *p) { struct uiparams *up=&p->up; struct gal_mesh_params *mp=&p->mp; struct gal_commonparams *cp=&p->cp; /* Print all the options that are set. Separate each group with a commented line explaining the options in that group. */ fprintf(fp, "\n# Input:\n"); if(cp->hduset) { if(gal_checkset_string_has_space(cp->hdu)) fprintf(fp, CONF_SHOWFMT"\"%s\"\n", "hdu", cp->hdu); else fprintf(fp, CONF_SHOWFMT"%s\n", "hdu", cp->hdu); } if(up->masknameset) { if(gal_checkset_string_has_space(up->maskname)) fprintf(fp, CONF_SHOWFMT"\"%s\"\n", "mask", up->maskname); else fprintf(fp, CONF_SHOWFMT"%s\n", "mask", up->maskname); } if(up->mhdu) { if(gal_checkset_string_has_space(up->mhdu)) fprintf(fp, CONF_SHOWFMT"\"%s\"\n", "mhdu", up->mhdu); else fprintf(fp, CONF_SHOWFMT"%s\n", "mhdu", up->mhdu); } if(up->kernelnameset) { if(gal_checkset_string_has_space(up->kernelname)) fprintf(fp, CONF_SHOWFMT"\"%s\"\n", "kernel", up->kernelname); else fprintf(fp, CONF_SHOWFMT"%s\n", "kernel", up->kernelname); } if(up->khdu) { if(gal_checkset_string_has_space(up->khdu)) fprintf(fp, CONF_SHOWFMT"\"%s\"\n", "khdu", up->khdu); else fprintf(fp, CONF_SHOWFMT"%s\n", "khdu", up->khdu); } fprintf(fp, "\n# Output:\n"); if(cp->outputset) fprintf(fp, CONF_SHOWFMT"%s\n", "output", cp->output); fprintf(fp, "\n# Mesh grid:\n"); if(up->meshsizeset) fprintf(fp, CONF_SHOWFMT"%zu\n", "meshsize", mp->meshsize); if(up->nch1set) fprintf(fp, CONF_SHOWFMT"%zu\n", "nch1", mp->nch1); if(up->nch2set) fprintf(fp, CONF_SHOWFMT"%zu\n", "nch2", mp->nch2); if(up->lastmeshfracset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "lastmeshfrac", mp->lastmeshfrac); if(up->mirrordistset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "mirrordist", mp->mirrordist); if(up->minmodeqset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "minmodeq", mp->minmodeq); if(up->numnearestset) fprintf(fp, CONF_SHOWFMT"%zu\n", "numnearest", mp->numnearest); if(up->smoothwidthset) fprintf(fp, CONF_SHOWFMT"%zu\n", "smoothwidth", mp->smoothwidth); if(up->fullconvolutionset) fprintf(fp, CONF_SHOWFMT"%d\n", "fullconvolution", mp->fullconvolution); if(up->fullinterpolationset) fprintf(fp, CONF_SHOWFMT"%d\n", "fullinterpolation", mp->fullinterpolation); if(up->fullsmoothset) fprintf(fp, CONF_SHOWFMT"%d\n", "fullsmooth", mp->fullsmooth); fprintf(fp, "\n# Statistics:\n"); if(up->sigclipmultipset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "sigclipmultip", p->sigclipmultip); if(up->sigcliptoleranceset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "sigcliptolerance", p->sigcliptolerance); /* For the operating mode, first put the macro to print the common options, then the (possible options particular to this program). */ fprintf(fp, "\n# Operating mode:\n"); GAL_CONFIGFILES_PRINT_COMMONOPTIONS; } /* Note that numthreads will be used automatically based on the configure time. */ void checkifset(struct subtractskyparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; int intro=0; if(cp->hduset==0) GAL_CONFIGFILES_REPORT_NOTSET("hdu"); if(up->khduset==0) GAL_CONFIGFILES_REPORT_NOTSET("khdu"); /* Mesh grid: */ if(up->meshsizeset==0) GAL_CONFIGFILES_REPORT_NOTSET("meshsize"); if(up->nch1set==0) GAL_CONFIGFILES_REPORT_NOTSET("nch1"); if(up->nch2set==0) GAL_CONFIGFILES_REPORT_NOTSET("nch2"); if(up->lastmeshfracset==0) GAL_CONFIGFILES_REPORT_NOTSET("lastmeshfrac"); if(up->mirrordistset==0) GAL_CONFIGFILES_REPORT_NOTSET("mirrordist"); if(up->minmodeqset==0) GAL_CONFIGFILES_REPORT_NOTSET("minmodeq"); if(up->numnearestset==0) GAL_CONFIGFILES_REPORT_NOTSET("numnearest"); if(up->smoothwidthset==0) GAL_CONFIGFILES_REPORT_NOTSET("smoothwidth"); if(up->fullconvolutionset==0) GAL_CONFIGFILES_REPORT_NOTSET("fullconvolution"); if(up->fullinterpolationset==0) GAL_CONFIGFILES_REPORT_NOTSET("fullinterpolation"); if(up->fullsmoothset==0) GAL_CONFIGFILES_REPORT_NOTSET("fullsmooth"); /* Statistics: */ if(up->sigclipmultipset==0) GAL_CONFIGFILES_REPORT_NOTSET("sigclipmultip"); if(up->sigcliptoleranceset==0) GAL_CONFIGFILES_REPORT_NOTSET("sigcliptolerance"); GAL_CONFIGFILES_END_OF_NOTSET_REPORT; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ void sanitycheck(struct subtractskyparams *p) { /* Make sure the input file exists. */ gal_checkset_check_file(p->up.inputname); /* Set the maskname and mask hdu accordingly: */ gal_fits_file_or_ext_name(p->up.inputname, p->cp.hdu, p->up.masknameset, &p->up.maskname, p->up.mhdu, p->up.mhduset, "mask"); /* Set the output name: */ if(p->cp.output) gal_checkset_check_remove_file(p->cp.output, p->cp.dontdelete); else gal_checkset_automatic_output(p->up.inputname, "_skysubed.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->cp.output); /* Set the sky image name: */ /* Set the check image names: */ if(p->meshname) { p->meshname=NULL; /* Was not allocated before! */ gal_checkset_automatic_output(p->up.inputname, "_mesh.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->meshname); } if(p->convname) { p->convname=NULL; /* Was not allocated before! */ gal_checkset_automatic_output(p->up.inputname, "_conv.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->convname); } if(p->skyname) { p->skyname=NULL; /* Was not allocated before! */ gal_checkset_automatic_output(p->up.inputname, "_sky.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->skyname); } /* Other checks: */ if(p->mp.numnearestmp.numnearest); /* Set the constants in the gal_mesh_params structure. */ p->mp.params=p; p->mp.numthreads=p->cp.numthreads; } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ void preparearrays(struct subtractskyparams *p) { struct gal_mesh_params *mp=&p->mp; /* Read the input image. */ gal_fits_file_to_float(p->up.inputname, p->up.maskname, p->cp.hdu, p->up.mhdu, (float **)&p->mp.img, &p->bitpix, &p->anyblank, &mp->s0, &mp->s1); gal_fits_read_wcs(p->up.inputname, p->cp.hdu, 0, 0, &p->nwcs, &p->wcs); /* Read the kernel: */ if(p->up.kernelnameset) gal_fits_prep_float_kernel(p->up.kernelname, p->up.khdu, &mp->kernel, &mp->ks0, &mp->ks1); /* Check if the input sizes and channel sizes are exact multiples. */ if( mp->s0%mp->nch2 || mp->s1%mp->nch1 ) error(EXIT_FAILURE, 0, "the input image size (%zu x %zu) is not an " "exact multiple of the number of the given channels (%zu, %zu) " "in the respective axis", mp->s1, mp->s0, mp->nch1, mp->nch2); } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void setparams(int argc, char *argv[], struct subtractskyparams *p) { struct gal_commonparams *cp=&p->cp; /* Set the non-zero initial values, the structure was initialized to have a zero value for all elements. */ cp->spack = SPACK; cp->verb = 1; cp->numthreads = num_processors(NPROC_CURRENT); cp->removedirinfo = 1; /* Read the arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Add the user default values and save them if asked. */ GAL_CONFIGFILES_CHECK_SET_CONFIG; /* Check if all the required parameters are set. */ checkifset(p); /* Print the values for each parameter. */ if(cp->printparams) GAL_CONFIGFILES_REPORT_PARAMETERS_SET; /* Do a sanity check. */ sanitycheck(p); /* Make the array of input images. */ preparearrays(p); /* Everything is ready, notify the user of the program starting. */ if(cp->verb) { printf(SPACK_NAME" started on %s", ctime(&p->rawtime)); printf(" - Using %zu CPU threads.\n", p->cp.numthreads); printf(" - Input: %s (hdu: %s)\n", p->up.inputname, p->cp.hdu); if(p->up.maskname) printf(" - Mask: %s (hdu: %s)\n", p->up.maskname, p->up.mhdu); if(p->up.kernelnameset) printf(" - Kernel: %s (hdu: %s)\n", p->up.kernelname, p->up.khdu); } } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void freeandreport(struct subtractskyparams *p, struct timeval *t1) { /* Free the allocated arrays: */ free(p->mp.img); free(p->cp.hdu); free(p->up.khdu); free(p->up.mhdu); free(p->cp.output); /* Free all the allocated names: */ if(p->meshname) free(p->meshname); if(p->up.kernelnameset) free(p->up.kernelname); /* Free the mask image name. Note that p->up.inputname was not allocated, but given to the program by the operating system. */ if(p->up.maskname && p->up.maskname!=p->up.inputname) free(p->up.maskname); /* Free the WCS structure: */ if(p->wcs) wcsvfree(&p->nwcs, &p->wcs); /* Print the final message. */ if(p->cp.verb) gal_timing_report(t1, SPACK_NAME" finished in: ", 0); } gnuastro-0.2.33-8a3b/bin/subtractsky/cite.h0000644000175000017500000000320512750745735015357 00000000000000/********************************************************************* SubtractSky - Find and subtract the sky value from an image. SubtractSky is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CITE_H #define CITE_H #define SUBTRACTSKYBIBTEX "" #define PRINTCITEABORT { \ printf("\nWe hope %s has been useful for your research.\n" \ "Citations are vital for the continued work on %s.\n" \ "Thank you for citing it in your research paper.\n" \ "\nPlease cite as \"%s\":\n\n%s\n\n%s", \ SPACK_NAME, SPACK_NAME, SPACK_STRING, \ GAL_STRINGS_MAIN_BIBTEX, SUBTRACTSKYBIBTEX); \ exit(EXIT_SUCCESS); \ } #endif gnuastro-0.2.33-8a3b/bin/subtractsky/main.h0000644000175000017500000000656412774161116015361 00000000000000/********************************************************************* SubtractSky - Find and subtract the sky value from an image. SubtractSky is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include #include #include /* Progarm name macros: */ #define SPACK "astsubtractsky" /* Subpackage executable name. */ #define SPACK_NAME "SubtractSky" /* Subpackage full name. */ #define SPACK_STRING SPACK_NAME" ("PACKAGE_NAME") "PACKAGE_VERSION struct uiparams { char *inputname; /* Name of input file. */ char *maskname; /* Name of mask image file. */ char *mhdu; /* Name of mask image header name. */ char *kernelname; char *khdu; int masknameset; int mhduset; int kernelnameset; int khduset; int numnearestset; int smoothwidthset; int mirrordistset; int minmodeqset; int fullconvolutionset; int fullinterpolationset; int fullsmoothset; int sigclipmultipset; int sigcliptoleranceset; int meshsizeset; int nch1set; int nch2set; int lastmeshfracset; }; struct subtractskyparams { /* Other structures: */ struct uiparams up; /* User interface parameters. */ struct gal_commonparams cp; /* Common parameters. */ struct gal_mesh_params mp; /* Mesh grid of input image. */ /* Input: */ int nwcs; /* Number of WCS structures. */ struct wcsprm *wcs; /* Pointer to WCS structures. */ int bitpix; /* Input image bitpix value. */ int anyblank; /* ==1: thereare blank pixels in input image. */ /* output: */ int checkstd; /* ==1: include the sky STD in checks. */ char *meshname; /* Name of --checkmesh output. */ char *convname; /* Name of --checkconvolution output. */ char *skyname; /* Name of sky and its STD image. */ /* Statistics: */ float sigclipmultip; /* Multiple of standard deviation, sigma clip. */ float sigcliptolerance; /* Tolerance in sigma clip. */ /* Operating mode: */ /* Internal: */ float *conv; /* Convolved input image. */ time_t rawtime; /* Starting time of the program. */ }; #endif gnuastro-0.2.33-8a3b/bin/subtractsky/main.c0000644000175000017500000000325712774160256015354 00000000000000/********************************************************************* SubtractSky - Find and subtract the sky value from an image. SubtractSky is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include /* Includes time.h and sys/time.h */ #include "main.h" #include "ui.h" /* needs main.h. */ #include "subtractsky.h" /* needs main.h. */ int main (int argc, char *argv[]) { struct timeval t1; struct subtractskyparams p={{0}, {0}, {0}, 0}; /* Set the starting time. */ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ setparams(argc, argv, &p); /* Run MakeProfiles */ subtractsky(&p); /* Free all non-freed allocations. */ freeandreport(&p, &t1); /* Return successfully.*/ return EXIT_SUCCESS; } gnuastro-0.2.33-8a3b/bin/subtractsky/Makefile.in0000644000175000017500000017266513004464627016337 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or 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GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ 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limit (for SysV at least) may be exceeded. .NOEXPORT: gnuastro-0.2.33-8a3b/bin/subtractsky/astsubtractsky.conf0000644000175000017500000000207712534316266020216 00000000000000# Default parameters (System) for SubtractSky. # SubtractSky is part of GNU Astronomy Utitlies. # # Use the long option name of each paramter followed by # a value. The name and value should be separated by # atleast one of the following charaacters: # space, `,`, `=` or `:` # # Run with `--help` option or read the manual for a full # explanation of what each option means. # # NOTE I: All counting is from zero, not one. # NOTE II: Lines starting with `#` are ignored. # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Input: hdu 0 khdu 0 # Output: # Mesh grid: meshsize 32 nch1 1 nch2 1 lastmeshfrac 0.6 numnearest 9 smoothwidth 5 fullconvolution 0 fullinterpolation 0 fullsmooth 0 # Statistics: mirrordist 1.5 minmodeq 0.49 sigclipmultip 3 sigcliptolerance 0.2gnuastro-0.2.33-8a3b/bin/subtractsky/Makefile.am0000644000175000017500000000272712765246727016331 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. NOTE: $(top_srcdir)/bootstrapped/lib is only necessary ## for internally compiled utilities and libraries. It must not be included ## during the tests since the bootstrapped libraries are not installed. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Utility and its sources bin_PROGRAMS = astsubtractsky astsubtractsky_SOURCES = main.c main.h cite.h ui.c ui.h args.h \ subtractsky.c subtractsky.h astsubtractsky_LDADD = $(top_builddir)/bootstrapped/lib/libgnu.la \ -lgnuastro ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astsubtractsky.conf gnuastro-0.2.33-8a3b/bin/noisechisel/0000755000175000017500000000000013004464725014257 500000000000000gnuastro-0.2.33-8a3b/bin/noisechisel/clumps.h0000644000175000017500000000665612764767045015705 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CLUMPS_H #define CLUMPS_H struct clumpsthreadparams { /* Main NoiseChisel parameters: */ struct noisechiselparams *p; /* Main NoiseChisel structure. */ /* Threads (only for detections, the noise uses the mesh threads.) */ size_t thislabel; /* The initial label of this detection. */ size_t id; /* ID of this thread. */ size_t *allareas; /* Array keeping the areas of all detections. */ size_t **alllabinds; /* Array of pointers to the indexs of all dets.*/ size_t *indexs; /* 2D array of initial indexs for each thread. */ pthread_barrier_t *b; /* pthreads barrier for running threads. */ pthread_mutex_t *totalnummtx; /* Mutex to change the total numbers. */ /* Box coordinates for this thread: */ size_t x0; /* Bottom left corner on x axis. */ size_t y0; /* Bottom left corner on y axis. */ size_t x1; /* Top right corner on x axis. */ size_t y1; /* Top right corner on y axis. */ /* Other basic parameters: */ float std; /* Standard deviation on this detection. */ size_t *topinds; /* Indexs of the top flux in each clump. */ size_t numclumps; /* Number of clumps in this set of pixels. */ size_t numobjects; /* Number of objects in this detected region. */ size_t area; /* Area of the current region for this thread. */ size_t *inds; /* Indexs of the current region for this thrd. */ size_t *blankinds; /* Array of pixels which should be grown. */ size_t numblanks; /* Number of blank pixels. */ long *segtoobjlabs; /* Convert from grown segments to object label.*/ long firstavailablelab; /* First free label over the full image. */ }; /* Important sizes and values (do not change). */ #define SEGMENTNOOBJ 0 #define SEGMENTMASKED -4 #define SEGMENTTMPCHECK -3 #define SEGMENTINIT -2 #define SEGMENTRIVER -1 #define INFOTABCOLS 5 #define WNGBSIZE 20 #define NOTOPIND (size_t)(-1) void oversegment(struct clumpsthreadparams *ctp); void growclumps(struct clumpsthreadparams *ctp, int withrivers); void clumpsntable(struct clumpsthreadparams *ctp, float **sntable); void findclumpsn(struct noisechiselparams *p); void removefalseclumps(struct clumpsthreadparams *ctp, float *sntable); #endif gnuastro-0.2.33-8a3b/bin/noisechisel/clumps.c0000644000175000017500000010633413001632540015642 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include "main.h" #include "clumps.h" #include "binary.h" #include "thresh.h" /**************************************************************** ***************** Over segmentation ******************** ****************************************************************/ /* This is very similar to the immersion method of Vincent & Soille(1991), but I will not separate the image into layers, and work based on the ordered flux values. If a certain pixel (at a certain level) has no neighbors it is a local maximum and will be assigned a new label. If it has a labeled neighbor, it will take that label and if there is more than one neighboring labeled region that pixel will be a `river` pixel. x0, y0, x1 and y1: - For the noise (mesh boxs), they specify the region in the image where this over-segmentation is taking place. - For the detections, they should be set to 0, 0, is0 and is1, where is0 and is1 are the height and width of the input image. */ void oversegment(struct clumpsthreadparams *ctp) { struct noisechiselparams *p=ctp->p; /* pix is not actually used its self, however, the pointer to it will be extensively used (ind) for the macro GAL_NEIGHBORS_FILL_8_REGION. This macro works on the pointer to the index, not the index its self. `pix` is filled with different index values, so the pointer to it doesn't change. */ size_t pix; float *arr=p->conv; struct gal_linkedlist_sll *Q=NULL, *cleanup=NULL; long n1, rlab, nlab, curlab=1, *clab=p->clab; size_t x0=ctp->x0, y0=ctp->y0, x1=ctp->x1, y1=ctp->y1; size_t *n, *nf, *indf, *pind, *ind=&pix, is1=p->lmp.s1; size_t ng, *rn, *rnf, numngb, ngb[8], *relngb=p->relngb; /* Sort the indexs based on the flux within them. */ qsort(ctp->inds, ctp->area, sizeof(size_t), gal_qsort_index_float_decreasing); /* Initialize the region you want to over-segment. */ indf=(pind=ctp->inds)+ctp->area; do clab[*pind]=SEGMENTINIT; while(++pindinds)+ctp->area; do /* When regions of a constant flux or masked regions exist, some later indexs (although they have same flux) will be filled before hand. If they are done, there is no need to do them again. */ if(clab[*pind]==SEGMENTINIT) { /* View the over-segmentation pixel by pixel. Make sure that `--viewsegtf` is off, or else several copies will be made. if(p->data0_noise1==0 && p->mid==81 && pind!=p->indexs) { long *tmp; float *ftmp; static size_t counter=0; size_t tmpx0=495, tmpy0=499, tmpx1=510, tmpy1=508; if(counter==0) { floatshrinkarraytonew(arr, np->lmesh.s0, np->lmesh.s1, tmpx0, tmpy0, tmpx1, tmpy1, &ftmp); array_to_fits("overseg.fits", NULL, "1", FLOAT_IMG, ftmp, tmpx1-tmpx0, tmpy1-tmpy0, NULL); free(ftmp); counter++; } if( *(pind-1)/is1>=tmpx0 && *(pind-1)/is1=tmpy0 && *(pind-1)%is1lmesh.s0, np->lmesh.s1, tmpx0, tmpy0, tmpx1, tmpy1, &tmp); array_to_fits("overseg.fits", NULL, "1", LONG_IMG, tmp, tmpx1-tmpx0, tmpy1-tmpy0, NULL); free(tmp); counter++; } } */ /* Some cases might happen where one or multiple regions of the pixels under study have the same flux. In particular note that masked pixels were all given a value of FLT_MAX. We have sorted the pixels by flux. So two equal valued pixels of two separate (but equal flux) regions might fall immediately after each other (For example two nearby stars whose centers are masked and are initially detected as one object because their wings touch above the noise). Therefore, if we see that the next pixel in the index list has the same flux as this one, it does not guarantee that it should be given the same label. Similar to the breadth first search algorithm for finding connected components, we will search all the neighbours and the neighbours of those neighbours that have the same flux of this pixel to see if they touch any label or not and to finally give them all the same label. */ if( pind+10) { if(n1==0) n1=nlab; else if(nlab!=n1) n1=SEGMENTRIVER; } /* If this neigbour has a label of zero, then we are on the edge of the region. When over-segmenting the noise and the detections, clab is zero for the parts of the image that we are not interested in (detections and noise respectively). */ else if(nlab==0) clab[*ind]=SEGMENTRIVER; } while(++ntopinds) ctp->topinds[rlab]=*pind; } /* Give the same label to the whole connected equal flux region, except those that might have been on the side of the image and were a river pixel. */ while(cleanup!=NULL) { gal_linkedlist_pop_from_sll(&cleanup, &pix); /* If it was on the sides of the image, it has been changed to a river pixel. */ if(clab[pix]==SEGMENTTMPCHECK) clab[pix]=rlab; } } /* The flux of this pixel is not the same as the next sorted flux, so simply find the label for this object. */ else { /* Check if the pixel is on the side of the image (for detections) or mesh box (for noise).*/ if(*pind/is1==x0 || *pind%is1==y0 || *pind/is1==x1-1 || *pind%is1==y1-1) n1=SEGMENTRIVER; else { /* Set the first neighbour's label to zero. */ n1=0; if(Q!=NULL || cleanup!=NULL) error(EXIT_FAILURE, 0, "a bug! Please contact us at %s " "so we can fix this problem. In oversegment " "(clumps.c) Q and cleanup should be NULL but while " "checking the equal flux regions they aren't", PACKAGE_BUGREPORT); /* Go over all the 8 neighbors of this pixel and see if all the neighbors that have a non-negative value belong to one label or not. If the pixel is neighboured by more than one label, set it as a river pixel. Also if it is touching a zero valued pixel (which does not belong to this object), set it as a river pixel. relngb was defined in ui.c: it keeps the relative indexs of the neighbors of a pixel.*/ rnf=(rn=relngb)+8; do { ng=*pind+*rn; nlab=clab[ng]; if(nlab>0) { if(n1==0) n1=nlab; else if(nlab!=n1) { n1=SEGMENTRIVER; break; } } else if(nlab==0) { n1=SEGMENTRIVER; break; } } while(++rntopinds ) ctp->topinds[rlab]=*pind; } /* Put the found label in the pixel. */ clab[ *pind ] = rlab; } } while(++pindnumclumps=curlab; } /******************************************************************/ /************* Grow clumps ******************/ /******************************************************************/ /* Grow the true clumps in a detection. Note that unlike before, were river pixels would get a separate label for them selves, here, they don't, they just get set back to SEGMENTINIT. This is because the some of the pixels that lie immediately between two labeled regions might not be in the blankinds array (they were below the threshold). So we have to find river pixels later on after the growth is done independently. */ void growclumps(struct clumpsthreadparams *ctp, int withrivers) { struct noisechiselparams *p=ctp->p; long n1, *olab=p->olab; size_t *ind, *indf, thisround, numngb; size_t *n, *nf, numblanks=ctp->numblanks; size_t ngb[8], is0=p->lmp.s0, is1=p->lmp.s1; /* It might happen that the growth threshold is larger than any of the non-clump pixels. So, if the number of blanks is zero, just leave this function. */ if(numblanks==0) return; /* The basic idea is this: after growing, not all the blank pixels are necessarily filled, for example the pixels might belong to two regions above the growth threshold. So the pixels in between them (which are below the threshold will not ever be able to get a label). Therefore, the safest way we can terminate the loop of growing the objects is to stop it when the number of pixels left to fill in this round (thisround) equals the number of blanks. To start the loop, we set thisround=numblanks+1. Note that immediately after the loop has started, thisround is set to numblanks, so we will not be reading an un-initialized element. */ thisround=numblanks+1; while(thisround>numblanks) { /* "thisround" will keep the number of pixels to be inspected in this round. "numblanks" will count the number of pixels left without an index by the end of this round. Since numblack comes from the previous loop (or outside for the first loop) it has to be saved in "thisround" to begin counting a fresh. */ thisround=numblanks; numblanks=0; /* Go over all the available indexs to fill: */ indf = ( ind=ctp->blankinds ) + thisround; do { /* We begin by assuming the neighbor label is zero (meaning that no neighbor actually exists!) */ n1=0; /* Check the 4 connected neighbors of the pixel: */ GAL_NEIGHBORS_FILL_4_ALLIMG; nf=(n=ngb)+numngb; do if( olab[*n]>0 ) /* This neighbor is labeled. */ { if(n1) /* A previous neighboring label was found. */ { if(n1!=olab[*n]) /* This neighbor has a new label. */ { /* So it should be set to SEGMENTINIT. */ n1=SEGMENTINIT; /* IMPORTANT: not SEGMENTRIVER. */ break; /* See explanations above. */ } } else /* This is the first labeled */ { /* neighbor that is found. */ n1=olab[*n]; if(!withrivers) break; } } while(++n No labeled neighbor was found. n1==SEGMENTINIT --> It is connecting two labeled regions. n1>0 --> It only has one neighbouring label.*/ if(n1==0) /* First condition above. */ ctp->blankinds[numblanks++]=*ind; else /* Last two conditions above. */ olab[*ind]=n1; } while(++indnumblanks=numblanks; } /******************************************************************/ /************* Clump S/N ******************/ /******************************************************************/ /* In this function we want to find the general information for each clump in an over-segmented labeled array. The signal in each clump is the average signal inside it subtracted by the average signal in the river pixels around it. So this function will go over all the pixels in the object (already found in deblendclumps()) and add them appropriately. The output is an array of size numseg*INFOTABCOLS. INFOTABCOLS=4. The columns are: 0: Average signal (flux) in clump. 1: Number of pixels in clump. 2: Average signal (flux) around clump. 3: Number of pixels around clump. 4: Standard deviation on flux weighted center of clump. */ void getclumpinfo(struct clumpsthreadparams *ctp, double **outclumpinfo) { struct noisechiselparams *p=ctp->p; struct gal_mesh_params *smp=&p->smp; double *xys, *clumpinfo; float *img=p->img, *smpstd=smp->garray2; size_t lab, is0=p->lmp.s0, is1=p->lmp.s1; long *clab=p->clab, wngb[WNGBSIZE], ngblab; size_t x0=ctp->x0, y0=ctp->y0, x1=ctp->x1, y1=ctp->y1; size_t i=0, ii=0, row, *n, *nf, ngb[8], *ind, *indf, numngb; /* Just make sure that the box size is not only around one pixel! */ if(x1-x0<=1 || y1-y0<=1) error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we can find " "and fix the problem in clumpinfo (clumps.c). For some reason, " "the specified input region is %zu by %zu wide", PACKAGE_BUGREPORT, y1-y0, x1-x0); /* Allocate the clump information array. */ errno=0; clumpinfo=calloc(ctp->numclumps*INFOTABCOLS, sizeof *clumpinfo); if(clumpinfo==NULL) error(EXIT_FAILURE, errno, "%zu bytes for clumpinfo in getclumpinfo " "(clumps.c)", ctp->numclumps*INFOTABCOLS*sizeof *clumpinfo); *outclumpinfo=clumpinfo; /* If the image is sky subtracted, we will need the light weighted center of each clump for finding the error in measuring the sky (through the smp->garray2). Since we are also segmenting the undetected regions, negative pixel values are common and they will mess up the flux weighted center (since all the weights have to be positive). So the xys array has three columns: the first is the total flux calculated from the positive pixels. The second is the x axis center and the third is the y axis center. */ if(p->skysubtracted) { errno=0; xys=calloc(3*ctp->numclumps, sizeof *xys); if(xys==NULL) error(EXIT_FAILURE, errno, "%zu bytes for xys (clumps.c)", 3*ctp->numclumps*sizeof *xys); } else xys=NULL; /* To check if it is needed below. */ /* Go over all the pixels in this set of pixels and fill in the proper information for each clump. */ indf = (ind=ctp->inds) + ctp->area; do if(!isnan(img[*ind])) { if(clab[*ind]==SEGMENTRIVER) /* We are on a river. */ { /* Fill in the neighbours arrary for this pixel. If we are working on the mesh grid (the noise), then we only want the neighbors within a region. Otherwise (when working on the detections) we want the neighbors on the full image.*/ if(p->b0f1) {GAL_NEIGHBORS_FILL_8_ALLIMG} else {GAL_NEIGHBORS_FILL_8_REGION} /* We are on a river pixel. So its value has to be added to the borders of any object it touches. But since it might touch a labeled region more than once, we use wngb to keep track of which label we have already added its value to. `ii` is the number of different labels this river pixel has already been added to. wngb will keep the labels. */ ii=0; memset(wngb, 0, sizeof(wngb)); /* Look into the 8-connected neighbors: */ nf=(n=ngb)+numngb; do if( (ngblab=clab[ *n ]) >0) { /* Go over wngb to see if this river pixel's value has been added to a segment or not. */ for(i=0;iskysubtracted && img[*ind]>0.0f) { xys[ 3 * lab ] += img[*ind]; xys[ 3 * lab + 1 ] += (*ind/is1) * img[*ind]; xys[ 3 * lab + 2 ] += (*ind%is1) * img[*ind]; } } } while(++indnumclumps;++lab) { row=lab*INFOTABCOLS; if(clumpinfo[row+1]>p->segsnminarea) { /* Find the index of the flux weighted center and use it to find the standard deviation for this clump. Note that this is only needed if the input image was already sky subtracted. If it wasn't, then we are not subtracting the sky to worry about its error! The error in a pixel flux measurement is simply its square root. */ if(p->skysubtracted) { /* Especially for noise, it might happen that no pixel within the clump was positive! If so, then the center cannot be calculated and the clump must not be used, so just set its area to zero. */ if(xys[3*lab]==0.0f) { clumpinfo[row+1]=0; continue; } else { xys[3*lab+1] /= xys[3*lab]; xys[3*lab+2] /= xys[3*lab]; if(p->skysubtracted) clumpinfo[row+4]= smpstd[gal_mesh_img_xy_to_mesh_id(smp,xys[3*lab+1], xys[3*lab+2])]; /* For a check: printf("%zu: (%zu, %zu) --> %f\n", lab, (size_t)(xys[3*lab+2] / clumpinfo[row]) +1, (size_t)(xys[3*lab+1] / clumpinfo[row]) +1, clumpinfo[row+4]); */ } } /* Convert sum to average. We are doing this after so if a clump should be ignored, control doesn't get to this point. */ clumpinfo[row ] /= clumpinfo[row+1]; clumpinfo[row+2] /= clumpinfo[row+3]; } } /* To check a specific detection (p->b0f1==1) or a noise mesh grid (p->b0f1==0). set ctp->thislabel to the desired label. if(p->b0f1==1 && ctp->thislabel==1) for(i=1;inumclumps;++i) printf("%zu: %-10.3f %-5.0f %-10.3f %-5.0f %-10.3f\n", i, clumpinfo[i*INFOTABCOLS], clumpinfo[i*INFOTABCOLS+1], clumpinfo[i*INFOTABCOLS+2], clumpinfo[i*INFOTABCOLS+3], clumpinfo[i*INFOTABCOLS+4]); */ /* If we are on the noise clumps, then xys is not needed any more. So if it was allocated, fre the space. */ if(p->skysubtracted) free(xys); } void clumpsntable(struct clumpsthreadparams *ctp, float **sntable) { struct noisechiselparams *p=ctp->p; float *sntab; double *clumpinfo, err; size_t i, ind, row, counter=0; double I, O, Ni, cpscorr=p->cpscorr; /* Get the information for all the segments. */ getclumpinfo(ctp, &clumpinfo); /* Allocate the signal to noise table. */ errno=0; sntab = *sntable = malloc( ctp->numclumps * sizeof *sntab ); if(sntab==NULL) error(EXIT_FAILURE, errno, "%zu bytes for sntab (clumps.c)", ctp->numclumps*sizeof *sntab); /* Start calculating the Signal to noise ratios. */ sntab[0]=0; for(i=1;inumclumps;++i) { /* These variables used for easy readability. */ row=i*INFOTABCOLS; I = clumpinfo[ row ]; Ni = clumpinfo[ row + 1 ]; O = clumpinfo[ row + 2 ]; /* If the inner flux is smaller than the outer flux (happens only in noise cases) or the area is smaller than the minimum area to calculate signal-to-noise, then set the S/N of this segment to zero. */ if( Ni>p->segsnminarea && I>O ) /* This is O, not 0 (zero). */ { /* If the sky was subtracted then put in the second power of the standard deviation multiplied by two (because we are measuring two fluxs). */ err = ( p->skysubtracted ? ( 2.0f * clumpinfo[row+4] * clumpinfo[row+4] ) : 0.0f ); /* Calculate the Signal to noise ratio, if we are on the noise regions, we don't care about the IDs of the clumps anymore, so store the Signal to noise ratios contiguously (for easy sorting and etc). Note that counter will always be smaller and equal to i. */ ind = p->b0f1 ? i : counter++; sntab[ind]=( sqrt((float)(Ni)/cpscorr)*(I-O) / sqrt( (I>0?I:-1*I) + (O>0?O:-1*O) + err ) ); } else sntab[i]=0; } /* If we are dealing with noise, replace the number of clumps with the number of those with a sufficient area and inner flux. */ if(p->b0f1==0) ctp->numclumps=counter; /* To check a specific detection (p->b0f1==1) or a noise mesh grid (p->b0f1==0): if(p->b0f1==1 && ctp->thislabel==151) { for(i=1;inumclumps;++i) printf("%zu: %-10.3g %-5.0f %-10.3g(%-5.0f) --> %-10.3g\n", i, clumpinfo[i*INFOTABCOLS], clumpinfo[i*INFOTABCOLS+1], clumpinfo[i*INFOTABCOLS+2], clumpinfo[i*INFOTABCOLS+3], sntab[i]); } */ /* Clean up */ free(clumpinfo); } /******************************************************************/ /************* S/N threshold ******************/ /******************************************************************/ void * clumpsntableonmesh(void *inparams) { struct clumpsthreadparams ctp; struct gal_mesh_thread_params *mtp=(struct gal_mesh_thread_params *)inparams; struct gal_mesh_params *mp=mtp->mp; struct noisechiselparams *p=(struct noisechiselparams *)mp->params; size_t *mponeforall=mp->oneforall; int anyblank; float *sntable; size_t s0, s1, nf, ind, startind, is1=mp->s1; size_t i, *indexs=&mp->indexs[mtp->id*mp->thrdcols]; /* Set the necessary pointers for the clumpsthreadparams structure. */ ctp.p=p; ctp.topinds=NULL; /* For noise, we don't want topinds. */ ctp.inds=&mponeforall[mtp->id*mp->maxs0*mp->maxs1]; /* Go over all the meshs that are assigned to this thread. */ for(i=0;indexs[i]!=GAL_THREADS_NON_THRD_INDEX;++i) { /* Set index of this mesh: */ ind=ctp.thislabel=indexs[i]; /* Find the necessary parameters */ startind=mp->start[ind]; s0=mp->ts0[mp->types[ind]]; s1=mp->ts1[mp->types[ind]]; ctp.x1 = (ctp.x0=startind/is1) + s0; ctp.y1 = (ctp.y0=startind%is1) + s1; /* Check to see if we have enough blank area for getting the background noise statistics. */ count_f_b_onregion(p->byt, startind, s0, s1, is1, &nf, &ctp.area, &anyblank); if( (float)ctp.area < (float)(s0*s1)*p->minbfrac ) { p->numclumpsarr[ind]=0; p->sntablearr[ind]=NULL; continue; } /* We want to find the clumps on the noise, not the signal, the number of noise pixels in this mesh were calculated above (area). Here we want to pull out the indexs of those pixels which is necessary for the over-segmentation. */ index_f_b_onregion(p->byt, startind, s0, s1, is1, ctp.inds, 0); /* Do the over-segmentation and put the number of clumps in ctp.numclumps */ oversegment(&ctp); /* Find the signal to noise of all the clumps. */ clumpsntable(&ctp, &sntable); /* Keep the relevant information for this mesh: */ p->sntablearr[ind]=sntable; p->numclumpsarr[ind]=ctp.numclumps; } /* Free any allocated space and if multiple threads were used, wait until all other threads finish. */ if(mp->numthreads>1) pthread_barrier_wait(&mp->b); return NULL; } /* The job of this function is to find the best signal to noise value to use as a threshold to detect real clumps. Each thread will find the useful signal to noise values for the meshs that have been assigned to it. It will then store the pointer to the S/N table into the sntablearr array (with the size of the number of meshs). If no clumps could be found in a mesh, then sntablearr[i]=NULL. Otherwise, it points to an array of the useful S/N values in that clump. Note that we don't care about the order of S/N values any more! There is also an accompanying array to keep the number of elements in the final S/N array of each mesh: numclumpsarr. Using these two arrays, after all the threads are finished, we can concatenate all the S/N values into one array and send it to the main findsnthresh function in thresh.c. */ void findclumpsn(struct noisechiselparams *p) { float *sntable; struct gal_mesh_params *lmp=&p->lmp; size_t i, j, numclumps=0, nmeshi=lmp->nmeshi; /* Set the convolved image as the basis for sorting the indexs and finding clumps. */ gal_qsort_index_arr=p->conv; /* Allocate the two arrays to keep the number and values of the S/Ns in each mesh. */ errno=0; p->numclumpsarr=malloc(nmeshi*sizeof*p->numclumpsarr); if(p->numclumpsarr==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->numclumpsarr in " "findclumpsn (clumps.c)", nmeshi*sizeof*p->numclumpsarr); errno=0; p->sntablearr=malloc(nmeshi*sizeof*p->sntablearr); if(p->sntablearr==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->sntablearr in " "findclumpsn (clumps.c)", nmeshi*sizeof*p->sntablearr); /* Find the clump Signal to noise ratio on successful meshs then on all the meshs. findsnthreshongrid is in detection.c. */ gal_mesh_operate_on_mesh(lmp, clumpsntableonmesh, sizeof(size_t), 0, 0); /* Find the total number of useful clumps and allocate sntable. */ for(i=0;inumclumpsarr[i]; errno=0; sntable=malloc(numclumps*sizeof*sntable); if(sntable==NULL) error(EXIT_FAILURE, errno, "%zu bytes for sntable in " "findclumpsn (clumps.c)", numclumps*sizeof*sntable); /* Fill in the sntable array: */ numclumps=0; for(i=0;inumclumpsarr[i];++j) sntable[numclumps++]=p->sntablearr[i][j]; /* Set the clump signal to noise value: */ snthresh(p, sntable, numclumps, 1); /* Clean up. In clumpsntableonmesh we put an allocated array in each member of p->sntablearr[i]. */ for(i=0;isntablearr[i]); free(p->numclumpsarr); free(p->sntablearr); free(sntable); } /******************************************************************/ /************* Remove false clumps ******************/ /******************************************************************/ /* Given the signal to noise of each segment (in sntable), and a threshold for an acceptable S/N (in `p`), remove those segments that don't satisfy the criteria and correct the number of clumps. */ void removefalseclumps(struct clumpsthreadparams *ctp, float *sntable) { struct gal_mesh_params *lmp=&ctp->p->lmp; long *newlabs, *clab=ctp->p->clab; size_t *n, *nf, is0=lmp->s0, is1=lmp->s1; size_t i, curlab=1, *ind, *indf, ngb[8], numngb; /* Allocate space for the new labels array. */ errno=0; newlabs=malloc(ctp->numclumps*sizeof *newlabs); if(newlabs==NULL) error(EXIT_FAILURE, errno, "%zu bytes for newlabs in " "removefalsedetections (clumps.c)", ctp->numclumps*sizeof *newlabs); /* We want the removed regions to become SEGMENTINIT. */ gal_array_long_init(newlabs, ctp->numclumps, SEGMENTINIT); /* Set the new labels: */ if(ctp->p->keepmaxnearriver) { /* `{' because We don't want to confuse the `else' below. */ for(i=1;inumclumps;++i) if( sntable[i] > ctp->p->clumpsn ) newlabs[i]=curlab++; } else for(i=1;inumclumps;++i) if(ctp->topinds[i]!=NOTOPIND) { /* Check to see if the brightest pixel in this clump is touching a river or not. */ ind=&ctp->topinds[i]; GAL_NEIGHBORS_FILL_8_ALLIMG; nf=(n=ngb)+numngb; do if(clab[*n++]==SEGMENTRIVER) break; while(n ctp->p->clumpsn ) newlabs[i]=curlab++; } ctp->numclumps=curlab; /* Change the values of the false clumps. Note that the labels are either SEGMENTRIVER or a label. */ indf = (ind=ctp->inds) + ctp->area; do { if(clab[*ind]>0) clab[*ind] = newlabs[ clab[*ind] ]; else clab[*ind] = SEGMENTINIT; } while(++ind Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef SEGMENTATION_H #define SEGMENTATION_H void clabwithnoseg(long *olab, long *clab, size_t size, int anyblank); void segmentation(struct noisechiselparams *p); #endif gnuastro-0.2.33-8a3b/bin/noisechisel/segmentation.c0000644000175000017500000006753313001632540017043 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include "main.h" #include "label.h" #include "clumps.h" #include "segmentation.h" /******************************************************************/ /***************** Growing preparations *******************/ /******************************************************************/ /* Set the growth threshold. We need one standard deviation for the full detection so we take the light weighted center of the full detected region and use that to find a standard deviation. Note that we are using the sky subtracted input image so gradients don't harm our results and that we only use pixels above the sky value. */ void prepfirstgrowth(struct clumpsthreadparams *ctp) { struct gal_mesh_params *smp=&ctp->p->smp; size_t *ind, *indf, is1=smp->s1; float growlimit, *imgss=ctp->p->imgss; double x=0.0f, y=0.0f, brightness=0.0f; long *olab=ctp->p->olab, *clab=ctp->p->clab; /* Try to find the flux weighted center (only on the pixels with positive flux) */ indf=(ind=ctp->inds)+ctp->area; do if(imgss[*ind]>0.0f) { brightness+=imgss[*ind]; x+=(*ind/is1)*imgss[*ind]; y+=(*ind%is1)*imgss[*ind]; } while(++indinds; do { x+=*ind/is1; y+=*ind%is1; } while(++indarea; y/=ctp->area; } else { x/=brightness; y/=brightness; } /* First find the standard deviation on this detection, then use it to calculate the growth threshold. */ ctp->std=smp->garray2[gal_mesh_img_xy_to_mesh_id(smp, x, y)]; growlimit=ctp->p->gthresh * ctp->std; /* Allocate and fill the array for the blank pixels and reset the olab pixels while you are at it. Note that after removing false clumps, usually most of the objects become blank, so we can just allocate an area the size of the detection: */ errno=0; ctp->blankinds=malloc(ctp->area*sizeof *ctp->blankinds); if(ctp->blankinds==NULL) error(EXIT_FAILURE, errno, "%zu bytes for ctp->blankpixels in " "prepfirstgrowth (clumps.c)", ctp->area*sizeof *ctp->blankinds); ctp->numblanks=0; indf=(ind=ctp->inds)+ctp->area; do { olab[*ind]=clab[*ind]; if(olab[*ind]==SEGMENTINIT && imgss[*ind]>growlimit) ctp->blankinds[ctp->numblanks++]=*ind; } while(++indp->olab; indf=(ind=ctp->inds)+ctp->area; do olab[*ind]=1; while(++indp->imgss; size_t numclumps=ctp->numclumps; long wngb[WNGBSIZE], *olab=ctp->p->olab; size_t i, j, ii, *n, *nf, ngb[8], numngb; double ave, rpave, c=sqrt(1/ctp->p->cpscorr); size_t *ind, *indf, is0=ctp->p->lmp.s0, is1=ctp->p->lmp.s1; double err=ctp->std*ctp->std*(ctp->p->skysubtracted?1.0f:2.0f); /* Go over all the still-unlabeled pixels and see which labels they touch. */ indf = (ind=ctp->inds) + ctp->area; do if( olab[*ind]==SEGMENTINIT && !isnan(imgss[*ind]) ) { /* Initialize the values to be used: */ ii=0; rpnum=1; rpave=imgss[*ind]; memset(wngb, 0, sizeof(wngb)); /* Find which grown clumps this river pixel touches. */ GAL_NEIGHBORS_FILL_8_ALLIMG; nf=(n=ngb)+numngb; do if( olab[*n]>0 ) { if(!isnan(imgss[*n])) /* Add the flux of this neighbor */ { /* pixel for finding the average */ ++rpnum; /* of this river pixel later. */ rpave+=imgss[*n]; } for(i=0;i1) { rpave/=rpnum; for(i=0;ithislabel==104) for(i=1;ip->olab; size_t i, j, ii, *ind, *indf; size_t numclumps=ctp->numclumps; /* Allocate the necessary arrays: */ errno=0; nums=calloc(numclumps*numclumps, sizeof *nums); if(nums==NULL) error(EXIT_FAILURE, errno, "%zu bytes for nums in grownclumpstoobjects " "(segmentation.c)", numclumps*numclumps*sizeof *nums); errno=0; sums=calloc(numclumps*numclumps, sizeof *sums); if(sums==NULL) error(EXIT_FAILURE, errno, "%zu bytes for sums in grownclumpstoobjects " "(segmentation.c)", numclumps*numclumps*sizeof *sums); errno=0; sns=calloc(numclumps*numclumps, sizeof *sns); if(sns==NULL) error(EXIT_FAILURE, errno, "%zu bytes for sns in grownclumpstoobjects " "(segmentation.c)", numclumps*numclumps*sizeof *sns); /* Find the signal to noise adjacency matrix for these grown clumps. */ adjacencymatrixs(ctp, sns, sums, nums); /* Remove the connections that are smaller than the required threshold. Note that we don't need to worry about the number of pixels, because each river pixels's value was the average of its self and its 8 neighbors. Note that these river pixels are also in systematically low valued regions, which is exactly what we want, so they aren't completely random and any area is important. Connections will be based on the `nums' array. So if a connection is severed, its place in nums will be set to zero. */ for(i=1;ip->minriverlength || sns[ii] < ctp->p->objbordersn ) nums[ ii ] = nums[ j*numclumps+i ]=0; /* Find the connected regions and assign new labels (starting from one) to the grown clumps regions. */ ctp->numobjects=BF_concomp_AdjMatrix(nums, numclumps, &ctp->segtoobjlabs); /* Correct all the pixels in olab: */ indf = (ind=ctp->inds) + ctp->area; do if(olab[*ind]>0) olab[*ind]=ctp->segtoobjlabs[ olab[*ind] ]; while(++indp->clab; size_t i, *ind, *indf, *numclumpsinobj; long *newclumplabs, *segtoobjlabs=ctp->segtoobjlabs; /* A simple sanity check. */ if(ctp->numclumps<=2 || ctp->numobjects<=2) error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we can fix " "it. For some reason, the newclumplabels function (in " "segmentation.c) was called for the %zu detected region, even " "though this region has ctp->numclumps=%zu and " "ctp->numobjects=%zu! This function should only be used when " "there is more than one object and clump over a detected region", PACKAGE_BUGREPORT, ctp->thislabel, ctp->numclumps, ctp->numobjects); /* 'numclumpsinobj' will keep the number of clumps in each object. Unlike the numbers of objects and clumps, this is the actual number of clumps in an object, NOT ADDED WITH ONE. */ errno=0; numclumpsinobj=calloc(ctp->numobjects, sizeof *numclumpsinobj); if(numclumpsinobj==NULL) error(EXIT_FAILURE, errno, "%zu bytes for numclumpsinobj in " "newclumplabels (segmentation.c)", ctp->numobjects*sizeof *numclumpsinobj); /* Allocate the array to keep the new clump labels. */ errno=0; newclumplabs=calloc(ctp->numclumps, sizeof *newclumplabs); if(newclumplabs==NULL) error(EXIT_FAILURE, errno, "%zu bytes for newclumplabs in " "newclumplabels (segmentation.c)", ctp->numclumps*sizeof *newclumplabs); /* Fill the newclumplabs and numclumpsinobj arrays: */ for(i=1;inumclumps;++i) newclumplabs[i]=++numclumpsinobj[ segtoobjlabs[i] ]; /* Reset the clump labels over the detected region */ indf=(ind=ctp->inds)+ctp->area; do if(clab[*ind]>0) clab[*ind]=newclumplabs[ clab[*ind] ]; while(++indp->grownclumps && ctp->numclumps<3) ? 1 : ctp->numclumps-1 ); /* If we are using multiple threads, lock the mutex, so only this thread can change the p->numobjects and p->numclumps values. */ if(ctp->p->cp.numthreads>1) pthread_mutex_lock(ctp->totalnummtx); ctp->firstavailablelab = ctp->p->numobjects; ctp->p->numobjects += ctp->numobjects-1; ctp->p->numclumps += numclumps; /* This thread is finished with the mutex, unlock it for the other threads: */ if(ctp->p->cp.numthreads>1) pthread_mutex_unlock(ctp->totalnummtx); } /******************************************************************/ /***************** Segmentation *******************/ /******************************************************************/ void * segmentonthread(void *inparam) { struct clumpsthreadparams *ctp=(struct clumpsthreadparams *)inparam; struct noisechiselparams *p=ctp->p; float *sntable; char *segmentationname=p->segmentationname; size_t i, *ind, *indf, s0=p->lmp.s0, s1=p->lmp.s1; /* For the detections, there is no box, only the sides of the image. */ ctp->x1=s0; ctp->y1=s1; ctp->x0=ctp->y0=0; /* Go over all the initial detections that were assigned to this thread. */ for(i=0;ctp->indexs[i]!=GAL_THREADS_NON_THRD_INDEX;++i) if(ctp->indexs[i]) /* sp->indexs[i]==0 for the background. */ { /* Keep the initial label of this detection. The initial label is mainly stored for possible debugging and checking. */ ctp->thislabel=ctp->indexs[i]; ctp->area=ctp->allareas[ctp->thislabel]; ctp->inds=ctp->alllabinds[ctp->thislabel]; /* Allocate the space for the indexs of the brightest pixels in each clump of this detection. We don't know how many clumps there are before hand, so to be safe just allocate a space equal to the number of pixels*/ errno=0; ctp->topinds=malloc(ctp->area*sizeof *ctp->topinds); if(ctp->topinds==NULL) error(EXIT_FAILURE, errno, "%zu bytes for ctp->topinds in " "segmentonthread (segmentation.c)", ctp->area*sizeof *ctp->topinds); /* Oversegment this detection. */ oversegment(ctp); if(segmentationname && p->stepnum==1) {free(ctp->topinds); continue;} /* Get the Signal to noise ratio of all the clumps within this detection. */ clumpsntable(ctp, &sntable); /* Remove clumps with smaller signal to noise ratios and free all the nolonger necessary arrays: */ removefalseclumps(ctp, sntable); free(ctp->topinds); free(sntable); if(segmentationname && p->stepnum==2) continue; /* Segmenting objects can only be defined when there is more than one segment. Since ctp->numclumps is the number of clumps+1, if an object has more than one clump, p->numclumps will be larger than two. When there is only one segment (p->numseg==2) or none (p->numseg==1), then just set the required preliminaries to make the next steps be generic for all cases. */ if(ctp->numclumps<=2) { ctp->numobjects=2; thisdetectionisoneobject(ctp); if(segmentationname && ( p->stepnum>=3 && p->stepnum<=6) ) continue; /* If the grown clumps are desired in the output, then replace all these grown clumps with those in p->clab. */ if(p->grownclumps) { indf=(ind=ctp->inds)+ctp->area; do p->clab[*ind]=p->olab[*ind]; while(++indstepnum==3) { free(ctp->blankinds); continue; } /* If the grown clumps are desired in the output, then replace all these grown clumps with those in p->clab. */ if(p->grownclumps) { indf=(ind=ctp->inds)+ctp->area; do p->clab[*ind]=p->olab[*ind]; while(++indnumobjects. This function allocates ctp->segtoobjlabs. */ grownclumpstoobjects(ctp); if(segmentationname && p->stepnum==4) { free(ctp->blankinds); free(ctp->segtoobjlabs); continue; } /* Fill in the full detected area. */ if(ctp->numclumps<=2) /* There is only one object in this whole detection. So automatically, the whole region should get a label of 1. Do that with this function. */ thisdetectionisoneobject(ctp); else { /* Grow the clumps unconditionally to fill the remaining blank pixels. */ ctp->numblanks=0; indf=(ind=ctp->inds)+ctp->area; do if(p->olab[*ind]<0) ctp->blankinds[ctp->numblanks++]=*ind; while(++indstepnum==5) { free(ctp->blankinds); free(ctp->segtoobjlabs); continue; } /* Set the final clump labels. Note that this is only necessary when there is more than object over the detection. When there is only one object over the full detection or if there is only one clump, the existing clump labels are fine. Note that both these counters are one more than the total number of objects or clumps (they are the labels of the next object). */ if(ctp->numobjects>2) newclumplabels(ctp); if(segmentationname && p->stepnum==6) { free(ctp->blankinds); free(ctp->segtoobjlabs); continue; } /* Clean up */ free(ctp->blankinds); free(ctp->segtoobjlabs); } /* Get the next available unique label for the final image. */ nextavailablelabel(ctp); /* Fix all the labels in the olab array */ indf=(ind=ctp->inds)+ctp->area; do p->olab[*ind] += ctp->firstavailablelab-1; while(++indcp.numthreads>1) pthread_barrier_wait(ctp->b); return NULL; } void segmentdetections(struct noisechiselparams *p, size_t numobjsinit, size_t *allareas, size_t **alllabinds) { int err; pthread_t t; /* We don't use the thread id, so all are saved here. */ pthread_attr_t attr; pthread_barrier_t b; pthread_mutex_t totalnummtx; struct clumpsthreadparams *ctp; size_t i, nb, *indexs, thrdcols; size_t numthreads=p->cp.numthreads; /* Allocate the arrays to keep the thread and parameters for each thread. */ errno=0; ctp=malloc(numthreads*sizeof *ctp); if(ctp==NULL) error(EXIT_FAILURE, errno, "%zu bytes in segmentdetections " "(segmentation.c) for ctp", numthreads*sizeof *ctp); /* Distribute the initial labels between all the threads. */ gal_threads_dist_in_threads(numobjsinit, numthreads, &indexs, &thrdcols); /* Spin off the threads to work on each object if more than one thread will be used. If not, simply start working on all the detections. */ if(numthreads==1) { ctp[0].p=p; ctp[0].id=0; ctp[0].indexs=indexs; ctp[0].allareas=allareas; ctp[0].alllabinds=alllabinds; segmentonthread(&ctp[0]); } else { /* Initialize the attributes. Note that this running thread (that spinns off the nt threads) is also a thread, so the number the barrier should be one more than the number of threads spinned off. */ if(numobjsinit0 ? SEGMENTINIT : 0 ) ); while(++olab0 ? SEGMENTINIT : 0 ; while(++olabsmp.s0, s1=p->smp.s1; char *segmentationname=p->segmentationname; size_t *labareas, **labinds, numobjsinit=p->numobjects; /* Start off the counter for the number of objects and clumps. The value to these variables will be the label that is given to the next clump or object found. Note that we stored a copy of the initial number of objects in the numobjsinit variable above.*/ p->numclumps=1; p->numobjects=1; /* Start the steps image: */ if(segmentationname) { gal_fits_array_to_file(segmentationname, "Input", FLOAT_IMG, p->img, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); gal_fits_array_to_file(segmentationname, "Convolved-SkySubtracted", FLOAT_IMG, p->conv, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); gal_fits_array_to_file(segmentationname, "InitialLabels", LONG_IMG, p->olab, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); } /* p->clab was used once during detection, we have to reset it to zero. Note that olab will be initialized for each object later on. Since we don't want to care about how clab was set an used, here we simply re-set all the blank pixels too. If there aren't any blank pixels, then just do a memset with no conditionals.*/ if(p->anyblank) { b=p->byt;lf=(l=p->clab)+s0*s1; do *l = *b++==GAL_FITS_BYTE_BLANK ? GAL_FITS_LONG_BLANK : 0; while(++lclab, 0, s0*s1*sizeof *p->clab); /* Find the true clump S/N threshold over the image. */ p->b0f1=0; findclumpsn(p); if(p->segmentationname) { gal_fits_array_to_file(p->segmentationname, "Noise Oversegmentaion", LONG_IMG, p->clab, p->smp.s0, p->smp.s1, p->anyblank, p->wcs, NULL, SPACK_STRING); } /* Initialize p->clab for the clumps within objects. */ if(p->anyblank) { lf=(l=p->clab)+s0*s1; do *l = *l==GAL_FITS_LONG_BLANK ? GAL_FITS_LONG_BLANK : 0; while(++lclab, 0, s0*s1*sizeof *p->clab); /* Save the indexs of all the detected labels. We will be working on each label independently: */ labindexs(p->olab, s0*s1, numobjsinit, &labareas, &labinds); /* Segment the detections. When the viewer wants to check the steps, the operations have to be repeated multiple times to output each step. */ p->b0f1=1; if(p->segmentationname) { p->stepnum=1; while(p->stepnum<8) { if(p->anyblank) { lf=(l=p->clab)+s0*s1; do *l = *l==GAL_FITS_LONG_BLANK ? GAL_FITS_LONG_BLANK : 0; while(++lclab, 0, s0*s1*sizeof *p->clab); segmentdetections(p, numobjsinit, labareas, labinds); switch(p->stepnum) { case 1: extname="Over-segmentation"; forfits=p->clab; break; case 2: extname="Successful clumps"; forfits=p->clab; break; case 3: extname="Clumps grown"; forfits=p->olab; break; case 4: extname="Objects found"; forfits=p->olab; break; case 5: extname="Objects grown"; forfits=p->olab; break; case 6: extname="New clump labels"; forfits=p->clab; break; case 7: extname="Final object labels"; forfits=p->olab; break; default: error(EXIT_FAILURE, 0, "a bug! Please contact us at %s to " "fix the problem. For some reason, the variable " "p->stepnum in segmenation (segmentation.c) has the " "unrecognized value of %d", PACKAGE_BUGREPORT, p->stepnum); } gal_fits_array_to_file(p->segmentationname, extname, LONG_IMG, forfits, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); ++p->stepnum; } } else segmentdetections(p, numobjsinit, labareas, labinds); /* Clean up */ for(i=0;i Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef SKY_H #define SKY_H void findavestdongrid(struct noisechiselparams *p, char *outname); void findsubtractskyconv(struct noisechiselparams *p); void subtractskyimg(struct noisechiselparams *p); #endif gnuastro-0.2.33-8a3b/bin/noisechisel/sky.c0000644000175000017500000002102412764767045015165 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include "main.h" #include "sky.h" void * avestdonthread(void *inparam) { struct gal_mesh_thread_params *mtp=(struct gal_mesh_thread_params *)inparam; struct gal_mesh_params *mp=mtp->mp; struct noisechiselparams *p=(struct noisechiselparams *)mp->params; float *mponeforall=mp->oneforall; float *oneforall=&mponeforall[mtp->id*mp->maxs0*mp->maxs1]; unsigned char *byt, *inbyt=p->byt; size_t s0, s1, ind, start, is1=mp->s1; float *f, *img, *imgend, *inimg=p->img; float ave, med, std, minbfrac=p->minbfrac; size_t i, num, row, *indexs=&mp->indexs[mtp->id*mp->thrdcols]; /* Start this thread's work: */ for(i=0;indexs[i]!=GAL_THREADS_NON_THRD_INDEX;++i) { /* Prepare the values: */ num=row=0; f=oneforall; ind=indexs[i]; start=mp->start[ind]; s0=mp->ts0[mp->types[ind]]; s1=mp->ts1[mp->types[ind]]; /* Copy all the non-NaN pixels images pixels of this mesh into the mesh array. Note that currently, the spatial positioning of the pixels is irrelevant, so we only keep those that are non-NaN. Recall that both the convolved an unconvolved image have the same NaN pixels.*/ do { byt = inbyt + start + row*is1; imgend=(img = inimg + start + row++ * is1 ) + s1; do /* Only input pixels that have byt==0 (note that NaN pixels have a non-zero byt value.) */ if(*byt++==0) { ++num; *f++ = *img; } while(++imgminbfrac ) { /* Sort the array of values: */ qsort(oneforall, num, sizeof *oneforall, gal_qsort_float_increasing); /* Do sigma-clipping and save the result if it is accurate. */ if(gal_statistics_sigma_clip_converge(oneforall, 1, num, p->sigclipmultip, p->sigcliptolerance, &ave, &med, &std, 0)) { mp->garray1[ind]=ave; mp->garray2[ind]=std; } } } /* Free any allocated space and if multiple threads were used, wait until all other threads finish. */ if(mp->numthreads>1) pthread_barrier_wait(&mp->b); return NULL; } /* Using the smaller mesh and the p->byt array, find the average and standard deviation of the undetected pixels and put them in the smp->garray1 and smp->garray2 arrays. This function will be used multiple times, the outputs for each should be different. So it takes the second argument as the name.*/ void findavestdongrid(struct noisechiselparams *p, char *outname) { struct gal_mesh_params *smp=&p->smp; size_t s0=smp->s0, s1=smp->s1; /* Find the average and standard deviation */ gal_mesh_operate_on_mesh(smp, avestdonthread, sizeof(float), 1, 1); if(outname) { if(smp->meshbasedcheck==0) gal_fits_array_to_file(outname, "Detected", BYTE_IMG, p->byt, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); gal_mesh_value_file(smp, outname, "Calculated Sky", "Calculated Sky STD", p->wcs, SPACK_STRING); } /* In case the image is in electrons or counts per second, the standard deviation of the noise will become smaller than unity. You have to find the minimum STD value (which is always positive) for later corrections. The maximum STD is only calculated here to include in the output headers so MakeCatalog can read it and not have to go through the whole STD array (which is the size of the full image for it). */ p->medstd=gal_statistics_median(smp->garray2, smp->nmeshi); gal_statistics_f_min_max(smp->garray2, smp->nmeshi, &p->minstd, &p->maxstd); p->cpscorr = p->minstd>1 ? 1.0f : p->minstd; /* Interpolate over the meshs to fill all the blank ones in both the sky and the standard deviation arrays: */ gal_mesh_interpolate(smp, "Interpolating sky value and its standard deviation"); if(outname) gal_mesh_value_file(smp, outname, "Interpolated Sky", "Interpolated Sky STD", p->wcs, SPACK_STRING); /* Smooth the interpolated array: */ if(smp->smoothwidth>1) { gal_mesh_smooth(smp); if(outname) gal_mesh_value_file(smp, outname, "Smoothed Sky", "Smoothed Sky STD", p->wcs, SPACK_STRING); } } /* Using the p->byt array find the sky value on the input and convolved images. Then subtract the sky value from both and save the standard deviation for every pixel in p->std. */ void findsubtractskyconv(struct noisechiselparams *p) { struct gal_mesh_params *smp=&p->smp; float *f, *fp, *tmpg1, *tmpg2, *tmpimg; size_t gid, s0, s1, row, start, chbasedid, is1=smp->s1; float csky, *tmpcg1, *tmpcg2, *tmpfg1, *tmpfg2, *convsky; /* Replace the necessary arrays to find the sky value on the convolved image. */ tmpimg=p->img; /* Keep backup pointers to the main arrays. */ tmpg1=smp->garray1; tmpg2=smp->garray2; tmpcg1=smp->cgarray1; tmpcg2=smp->cgarray2; tmpfg1=smp->fgarray1; tmpfg2=smp->fgarray2; p->img=smp->img=p->conv; /* Prepare for working on convolved image. */ smp->cgarray1=smp->cgarray2=NULL; smp->fgarray1=smp->fgarray2=NULL; findavestdongrid(p, NULL); convsky=smp->garray1; /* Keep garray1, free the rest. */ if(smp->garray1==smp->cgarray1) free(smp->fgarray1); else free(smp->cgarray1); free(smp->cgarray2); free(smp->fgarray2); p->img=smp->img=tmpimg; /* Set back to their previous state */ smp->garray1=tmpg1; smp->garray2=tmpg2; smp->cgarray1=tmpcg1; smp->cgarray2=tmpcg2; smp->fgarray1=tmpfg1; smp->fgarray2=tmpfg2; /* Subtract the sky */ for(gid=0;gidnmeshi;++gid) { /* Get the meshid from i: */ chbasedid=gal_mesh_ch_based_id_from_gid(smp, gid); /* Subtract the sky for each pixel. */ row=0; csky = convsky[gid]; start=smp->start[chbasedid]; s0=smp->ts0[smp->types[chbasedid]]; s1=smp->ts1[smp->types[chbasedid]]; do { fp= ( f = p->conv + start + row++ * is1 ) + s1; do *f++ -= csky; while(fsmp; float *f, *fp, *in, sky; size_t gid, s0, s1, row, start, chbasedid, is1=smp->s1; /* Apply the threshold */ for(gid=0;gidnmeshi;++gid) { /* Get the meshid from i: */ chbasedid=gal_mesh_ch_based_id_from_gid(smp, gid); /* Subtract the sky for each pixel. */ row=0; sky = smp->garray1[gid]; start=smp->start[chbasedid]; s0=smp->ts0[smp->types[chbasedid]]; s1=smp->ts1[smp->types[chbasedid]]; do { in = p->img + start + row * is1; fp= ( f = p->imgss + start + row++ * is1 ) + s1; do *f = *in++ - sky; while(++f Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef DETECTION_H #define DETECTION_H void initialdetection(struct noisechiselparams *p); void onlytruedetections(struct noisechiselparams *p); #endif gnuastro-0.2.33-8a3b/bin/noisechisel/detection.c0000644000175000017500000005263313001632540016317 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include "main.h" #include "sky.h" #include "label.h" #include "thresh.h" #include "binary.h" #include "detection.h" /**************************************************************** ************ Initial detection ************ ****************************************************************/ void initialdetection(struct noisechiselparams *p) { int verb=p->cp.verb; size_t i, s0=p->smp.s0, s1=p->smp.s1; char *detectionname=p->detectionname; char report[GAL_TIMING_VERB_MSG_LENGTHS_2_V]; /* Find the threshold and apply it, if there are blank pixels in the image, set those pixels to the binary blank value too: */ findapplyqthreshold(p); if(detectionname) gal_fits_array_to_file(detectionname, "Thresholded", BYTE_IMG, p->byt, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); if(verb) { sprintf(report, "%.2f quantile threshold found and applied.", p->qthresh); gal_timing_report(NULL, report, 2); } /* Erode the thresholded image, then convert the pixels that should not have been eroded back to 1 so the next step (opening) can be completely ignorant of them. */ if(p->erodengb==4) for(i=0;ierode;++i) dilate0_erode1_4con(p->byt, s0, s1, 1); else for(i=0;ierode;++i) dilate0_erode1_8con(p->byt, s0, s1, 1); gal_array_uchar_replace(p->byt, s0*s1, BINARYNOOP, 1); if(detectionname) gal_fits_array_to_file(detectionname, "Eroded", BYTE_IMG, p->byt, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); if(verb) { sprintf(report, "Eroded %zu times (%s connectivity).", p->erode, p->erodengb==4 ? "4" : "8"); gal_timing_report(NULL, report, 2); } /* Do the opening: */ opening(p->byt, s0, s1, p->opening, p->openingngb); if(detectionname) gal_fits_array_to_file(detectionname, "Opened", BYTE_IMG, p->byt, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); if(verb) { sprintf(report, "Opened (depth: %zu, %s connectivity).", p->opening, p->openingngb==4 ? "4" : "8"); gal_timing_report(NULL, report, 2); } /* Label the connected regions. Note that p->olab was allocated in ui.c and will be freed there. */ p->numobjects=BF_concmp(p->byt, p->olab, s0, s1, p->anyblank, 4); if(detectionname) gal_fits_array_to_file(detectionname, "Labeled", LONG_IMG, p->olab, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); } /**************************************************************** ********* Signal to noise ratio calculation ************ ****************************************************************/ /* Calculate the Signal to noise ratio for all the labels in p->clab which is keeping all the pseudo detections' labels. However, the array keeping the labels of each object is only over the mesh under consideration. */ void detlabelsn(struct noisechiselparams *p, size_t *numlabs, float **outsntable) { float *imgss=p->imgss; struct gal_mesh_params *smp=&p->smp; double *brightnesses, err, *xys; float *f, *ff, ave, *sntable, cpscorr=p->cpscorr; size_t i, ind, xyscol=3, is1=p->smp.s1, counter=0; unsigned char *coversdet=NULL, b0f1=p->b0f1, *b=p->byt; long *areas, *lab=p->clab, *lf, detsnminarea=p->detsnminarea; /* Allocate the necessary arrays to keep the label information: */ errno=0; sntable=*outsntable=calloc(*numlabs, sizeof *sntable); if(sntable==NULL) error(EXIT_FAILURE, errno, "%zu bytes for sntable in detlabelsn " "(detection.c)", *numlabs*sizeof *sntable); errno=0; brightnesses=calloc(*numlabs, sizeof *brightnesses); if(brightnesses==NULL) error(EXIT_FAILURE, errno, "%zu bytes for brightnesses in detlabelsn " "(detection.c)", *numlabs*sizeof *brightnesses); errno=0; xys=calloc(*numlabs*xyscol, sizeof *xys); if(xys==NULL) error(EXIT_FAILURE, errno, "%zu bytes for xys in detlabelsn " "(detection.c)", *numlabs*sizeof *xys); errno=0; areas=calloc(*numlabs, sizeof *areas); if(areas==NULL) error(EXIT_FAILURE, errno, "%zu bytes for areas in detlabelsn " "(detection.c)", *numlabs*sizeof *areas); if(b0f1==0) { errno=0; coversdet=calloc(*numlabs, sizeof *coversdet); if(coversdet==NULL) error(EXIT_FAILURE, errno, "%zu bytes for coversdet in detlabelsn " "(detection.c)", *numlabs*sizeof *coversdet); } /* Go over the area and fill in the necessary information for calculating the Signal to noise ratio. */ ff = (f=imgss) + p->smp.s0*p->smp.s1; do { /* See label.h for this macro. It checks speciie*/ if(ISINDEXABLELABEL) { /* This test is done first so if the sky region pseudo-detection lies over a detected object it doesn't waste our time for the next calculations. */ if(b0f1==0) { if(coversdet[*lab]) {++lab; ++b; continue;} else if(*b==1) {coversdet[*lab]=1; areas[*lab]=0; ++lab; ++b; continue;} } if(isnan(*f)) error(EXIT_FAILURE, 0, "*f was nan"); ++areas[*lab]; brightnesses[*lab] += *f; if(f-imgss>0) { xys[*lab*xyscol+2] += f-imgss; xys[*lab*xyscol ] += (double)((f-imgss)/is1) * *f; xys[*lab*xyscol+1] += (double)((f-imgss)%is1) * *f; } } ++lab; if(b0f1==0) ++b; } while(++fdetectionname && b0f1==0) { b=p->dbyt; lf=(lab=p->clab)+p->smp.s0*p->smp.s1; do { if( ISINDEXABLELABEL && (areas[*lab]detectionname, "For S/N", BYTE_IMG, p->dbyt, p->smp.s0, p->smp.s1, p->anyblank, p->wcs, NULL, SPACK_STRING); } /* calculate the signal to noise for successful detections: */ for(i=1;i<*numlabs;++i) { ave=brightnesses[i]/areas[i]; if(areas[i]>detsnminarea && ave>0.0f && xys[i*xyscol+2]>0.0f) { /* Find the flux weighted center of this object in each dimension to find the mesh it belongs to and get the standard deviation at this point. Note that the standard deviation on the grid was stored in smp->garray2. The error should then be taken to the power of two and if the sky is subtracted, a 2 should be multiplied to it.*/ err = smp->garray2[ gal_mesh_img_xy_to_mesh_id(smp, xys[i*xyscol]/xys[i*xyscol+2], xys[i*xyscol+1]/xys[i*xyscol+2]) ]; err *= p->skysubtracted ? err : 2.0f*err; /* Set the index in the sntable to store the Signal to noise ratio. When we are dealing with the noise, we only want the non-zero signal to noise values, so we will just use a counter. But for initial detections, it is very important that their Signal to noise ratio be placed in the same index as their label. */ ind = p->b0f1 ? i : counter++; sntable[ind] = ( sqrt( (float)(areas[i])/cpscorr ) * ave / sqrt(ave+err) ); } } /* In background mode, set the number of labels to the number of acceptable S/N values measured. */ if(p->b0f1==0) *numlabs=counter; /* For a check. IMPORTANT NOTE: in background mode, the sntable is not ordered like the areas, brightnesses and coversdet arrays. Since indexes are irrelevant for this mode, they are just put contigusly in memory for the next step. if(b0f1) { for(i=0;i<*numlabs;++i) printf("%zu: %-10ld %-10.3f %-10.3f\n", i, areas[i], brightnesses[i], sntable[i]); } */ /* Clean up */ free(xys); free(areas); free(brightnesses); if(b0f1==0) free(coversdet); } /* Apply the S/N threshold on the pseudo-detections. */ void applydetsn(struct noisechiselparams *p, float *sntable, size_t numpseudo) { size_t i, curlab=1; unsigned char *b=p->dbyt; long *newlabs, *lab, *lf, *clab=p->clab; errno=0; newlabs=calloc(numpseudo, sizeof *newlabs); if(newlabs==NULL) error(EXIT_FAILURE, errno, "%zu bytes for numlabs in " "removefalsedetections (detections.c)", numpseudo*sizeof *newlabs); for(i=1;i p->detsn) newlabs[i]=curlab++; lf= (lab=clab) + p->smp.s0*p->smp.s1; do { if(*lab!=GAL_FITS_LONG_BLANK) *b = newlabs[*lab] > 0; ++b; } while(++labdetectionname) gal_fits_array_to_file(p->detectionname, "True pseudo-detections", BYTE_IMG, p->dbyt, p->smp.s0, p->smp.s1, p->anyblank, p->wcs, NULL, SPACK_STRING); free(newlabs); } /**************************************************************** ************ Remove false detections ************ ****************************************************************/ /* The p->byt points to the array keeping the positions of initial detections. p->dbyt points to the array keeping the thresholded values for removal of false detections. We want to copy the above threshold (with value 1) parts of p->dbyt to `out' which are either foreground or background in p->byt (depending on if the process is done over the detections or over the noise). */ void bytpartfromlarge(struct noisechiselparams *p, unsigned char *out, size_t start, size_t s0, size_t s1) { size_t r=0, is1=p->smp.s1; unsigned char *b, *d, *bf, b0f1=p->b0f1; do { d = p->dbyt + start + r*is1; bf = ( b = p->byt + start + r++ * is1 ) + s1; do { *out++ = *b==b0f1 ? *d : (*b==GAL_FITS_BYTE_BLANK ? GAL_FITS_BYTE_BLANK : 0); ++d; } while(++bsmp.s1; do { df = ( d = p->dbyt + start + r++ * is1 ) + s1; do *d=*in++; while(++dmp; struct noisechiselparams *p=(struct noisechiselparams *)mp->params; unsigned char *mponeforall=mp->oneforall; unsigned char *thisbyt=&mponeforall[mtp->id*mp->maxs0*mp->maxs1]; int anyblank; size_t i, s0, s1; unsigned char *b, *bf; size_t ind, startind; char *detectionname=p->detectionname; size_t *indexs=&mp->indexs[mtp->id*mp->thrdcols]; /* Do the job for each mesh: */ for(i=0;indexs[i]!=GAL_THREADS_NON_THRD_INDEX;++i) { /* Set the necesary parameters: */ ind=indexs[i]; s0=mp->ts0[mp->types[ind]]; s1=mp->ts1[mp->types[ind]]; startind=mp->start[ind]; anyblank=0; /* Copy this mesh into a separate array. In the meantime, only bring in the desired pixels. If the user wanted to see the steps, then save the result to the p->dbyt and come leave the work for this mesh if this is the first step. */ bytpartfromlarge(p, thisbyt, startind, s0, s1); if(detectionname && p->stepnum==1) { bytparttolarge(p, thisbyt, startind, s0, s1); continue; } /* If there were NaN pixels in the image, make sure if this mesh has any or not. */ if(p->anyblank) { bf=(b=thisbyt)+s0*s1; do if(*b++==GAL_FITS_BYTE_BLANK) { anyblank=1; break; } while(bstepnum==2) { bytparttolarge(p, thisbyt, startind, s0, s1); continue; } /* Open the image once: */ opening(thisbyt, s0, s1, 1, 4); /* Put this region back into p->dbyte. */ bytparttolarge(p, thisbyt, startind, s0, s1); } /* If multiple threads were used, wait until all other threads finish. */ if(mp->numthreads>1) pthread_barrier_wait(&mp->b); return NULL; } /* Doing object detection is done separately on each mesh both for the first part of finding the SN limit and the second part of applying it and removing false detections. Therefore, if the user asks to view the steps, the mesh process has to be stopped at differnt times for all the meshs and re-done for each step. This function does that job. Here we temporarily (clab will be cleaned when it is needed) operate on the p->clab array which is finally used to keep the clump labels. */ void detsnthresh(struct noisechiselparams *p) { struct gal_mesh_params *lmp=&p->lmp; float *sntable; static int b0f1; char *extname=NULL; unsigned char *tmp, *originaldbyt; size_t numpseudo, s0=lmp->s0, s1=lmp->s1; /* General preparations: */ p->b0f1 = b0f1++; /* All the operations below happen on p->dbyt, but we need it two times (once for the sky region and once for the detected region). So the first time we operate on it, */ if(p->b0f1==0) gal_array_uchar_copy(p->dbyt, s0*s1, &originaldbyt); /* Find the psudo-detections: */ if(p->detectionname) { p->stepnum=1; /* Backup of p->dbyt in tmp */ gal_array_uchar_copy(p->dbyt, s0*s1, &tmp); while(p->stepnum<4) { free(p->dbyt); /* Free the old, p->dbyt, put the original */ gal_array_uchar_copy(tmp, s0*s1, &p->dbyt); gal_mesh_operate_on_mesh(lmp, detectpseudos, sizeof(unsigned char), 0, 0); switch(p->stepnum) { case 1: extname = p->b0f1 ? "ThresholdDetections" : "ThresholdNoise"; break; case 2: extname="HolesFilled"; break; case 3: extname="Opened"; break; default: error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we " "can find the solution. For some reason, the value to " "p->stepnum (%d) is not recognized in detsnthresh " "(detection.c)", PACKAGE_BUGREPORT, p->stepnum); } gal_fits_array_to_file(p->detectionname, extname, BYTE_IMG, p->dbyt, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); ++p->stepnum; } free(tmp); } else gal_mesh_operate_on_mesh(lmp, detectpseudos, sizeof(unsigned char), 0, 0); /* Find the connected components and the signal to noise ratio of all the detections. Note that when dealing with the background pixels in p->byt, the order of sntable is no longer valid, since we don't care any more, we just want their sorted values for the quantile. */ numpseudo=BF_concmp(p->dbyt, p->clab, s0, s1, p->anyblank, 4); if(p->detectionname) gal_fits_array_to_file(p->detectionname, "Labeled", LONG_IMG, p->clab, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); detlabelsn(p, &numpseudo, &sntable); /* Find or apply the threshold depending on if we are dealing with the background or foreground. */ if(p->b0f1) applydetsn(p, sntable, numpseudo); else { snthresh(p, sntable, numpseudo, 0); free(p->dbyt); p->dbyt=originaldbyt; } /* Clean up: */ free(sntable); } void dbytolaboverlap(struct noisechiselparams *p) { unsigned char *byt; long *lf, *tokeep, *lab; size_t numobjects=p->numobjects; size_t i, size=p->smp.s0*p->smp.s1, curlab=1; /* Allocate array to keep the overlapping labels. */ errno=0; tokeep=calloc(numobjects, sizeof*tokeep); if(tokeep==NULL) error(EXIT_FAILURE, errno, "%zu bytes for tokeep in dbytolaboverlap " "(detection.c)", numobjects*sizeof*tokeep); /* Note that the zeroth element of tokeep can also be non zero, this is because the holes of the labeled regions might be filled during filling the holes, but have not been filled in the original labeled array. They are not important so you can just ignore them. The basic idea is that after the first pixel of a label overlaps with dbyt[i], we don't need to check the rest of that object's pixels. At this point, tokeep is only binary: 0 or 1. */ byt=p->dbyt; lf=(lab=p->olab)+size; do { if(ISINDEXABLELABEL) { tokeep[ *lab ] = tokeep[ *lab ] /* Check if this label is to be kept. */ ? 1 /* It has, its all we need! */ : *byt; /* It hasn't, check if it should be kept.*/ } ++byt; } while(++labbyt; lf=(lab=p->olab)+size; if(p->dilate) do { if(*lab!=GAL_FITS_LONG_BLANK) *byt=tokeep[*lab]>0; ++byt; } while(++lab 0; ++byt; } while(++labnumobjects=curlab; free(tokeep); } /*********************************************************************/ /************** Main detection function *******************/ /*********************************************************************/ void onlytruedetections(struct noisechiselparams *p) { struct gal_mesh_params *lmp=&p->lmp; int verb=p->cp.verb; char report[GAL_TIMING_VERB_MSG_LENGTHS_2_V]; char *detectionname=p->detectionname; size_t s0=lmp->s0, s1=lmp->s1, numobjects=p->numobjects; /* Find the average and STD of the undetected pixels for each mesh for the initial detection threshold: */ findavestdongrid(p, p->detectionskyname); /* Apply the false detection removal threshold to the image. */ applydetectionthresholdskysub(p); if(detectionname) gal_fits_array_to_file(detectionname, "InitalSkySubtracted", FLOAT_IMG, p->imgss, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); if(verb) { sprintf(report, "Initial sky threshold (%.3f sigma) applied.", p->dthresh); gal_timing_report(NULL, report, 2); } /* Find the Signal to noise ratio threshold on the grid and keep it in one array. */ detsnthresh(p); /* Apply the SN threshold to all the detections. */ detsnthresh(p); /* Select the true detections: */ dbytolaboverlap(p); if(detectionname) gal_fits_array_to_file(detectionname, "TrueDetections", BYTE_IMG, p->byt, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); if(verb) { /* p->numobjects changed in dbytlaboverlap. */ sprintf(report, "%zu false detections removed.", numobjects-p->numobjects); gal_timing_report(NULL, report, 2); } /* Clean up: */ free(p->dbyt); } gnuastro-0.2.33-8a3b/bin/noisechisel/label.h0000644000175000017500000000421112750745735015437 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef LABEL_H #define LABEL_H /* For the GAL_FITS_LONG_BLANK and GAL_FITS_BYTE_BLANK macros: */ #include /* In case the blank value for the long type is negative, the only necessary check to see if we are on a label or not is to see if its value is positive. But since we don't want to impose this condition on the fits.h macro (which is used by all Gnuastro programs) we allow for it to be positive through this C preprocessor check. The compiler has no idea of our convention to label things with positive indices, so we can't rely on the compiler to optimize this. */ #if GAL_FITS_LONG_BLANK<0 #define ISINDEXABLELABEL (*lab>0) #else #define ISINDEXABLELABEL (*lab && *lab!=GAL_FITS_LONG_BLANK) #endif size_t BF_concmp(unsigned char *byt, long *lab, size_t s0, size_t s1, int anyblank, const size_t connectivity); size_t BF_concomp_AdjMatrix(int *adj, size_t numside, long **outnewlabs); void removesmallarea_relabel(long *in, unsigned char *byt, size_t size, size_t *numlabs, size_t minarea); void labindexs(long *lab, size_t size, size_t numlabs, size_t **outareas, size_t ***outlabinds); #endif gnuastro-0.2.33-8a3b/bin/noisechisel/label.c0000644000175000017500000002775613002706670015437 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include "main.h" #include "label.h" #include "binary.h" /**********************************************************************/ /************** Connected component labeling *******************/ /**********************************************************************/ /* Find the connected components in an image based on the breadth first algorithm. The output curlab is one more than the actual number of objects in the array. The input image is a unsigned char binary, either background (==0) or foreground (==1), image. This function will find and label the different components of all pixels labeled b0_f1.*/ size_t BF_concmp(unsigned char *byt, long *lab, size_t s0, size_t s1, int anyblank, const size_t connectivity) { struct gal_linkedlist_sll *Q=NULL; long *l=lab, curlab=1; /* Current label */ size_t i, p, size=s0*s1, s0t1=s0-1, s1t1=s1-1; unsigned char *b=byt, *bf=byt+s0*s1, counter, bl, br, tl, tr; /* A simple sanity check. */ if(connectivity!=4 && connectivity!=8) error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we can fix " "the problem. For some reason, the value to connectivity in " "BF_concmp (label.c) is %zu which is not recognized", PACKAGE_BUGREPORT, connectivity); /* Initialize the labels array. If we have blank pixels in the byt array, then give them the blank labeled array. Note that since their value will not be 0, they will also not be labeled. */ if(anyblank) do *l++ = *b==GAL_FITS_BYTE_BLANK ? GAL_FITS_LONG_BLANK : 0; while(++b0 && byt[p-s1] && !lab[p-s1]) {gal_linkedlist_add_to_sll(&Q, p-s1); lab[p-s1]=curlab;} if(p/s10 && byt[p-1] && !lab[p-1]) {gal_linkedlist_add_to_sll(&Q, p-1); lab[p-1]=curlab;} if(p%s10) { ++counter; ++bl; ++br; if(byt[p-s1] && !lab[p-s1]) {gal_linkedlist_add_to_sll(&Q, p-s1); lab[p-s1]=curlab;} } if(p/s10) { ++counter; ++bl; ++tl; if(byt[p-1] && !lab[p-1]) {gal_linkedlist_add_to_sll(&Q, p-1); lab[p-1]=curlab;} } if(p%s1minarea) newlabs[i]=curlab++; if(byt) { for(i=0;i 0; } else { for(i=0;i Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef BINARY_H #define BINARY_H /* For the GAL_FITSARRAY_BYTE_BLANK value: */ #include /* Special values: BINARYNOOP: Value that no binary operation should be preformed on. BINARYTMP: Temporary value to use within one function. Note that through the `setbytblank' function, practically we are using the value `GAL_FITS_BYTE_BLANK' (from `gnuastro/fits.h') for blank binary values. Recall that due to the nature of the CPU (which operates on 8-bits), in practice it is much more efficient to work on a byte (or 8-bits) rather than each bit. So in practice we can use 256 values for meta-data analyais (like blank values, or temporary values at etc), eventhough the main values we are working with are 0 and 1. */ #define BINARYNOOP 2 #define BINARYTMP 3 void setbytblank(float *img, unsigned char *byt, size_t size); void count_f_b_onregion(unsigned char *byt, size_t startind, size_t s0, size_t s1, size_t is1, size_t *numf, size_t *numb, int *anyblank); void index_f_b_onregion(unsigned char *byt, size_t startind, size_t s0, size_t s1, size_t is1, size_t *inds, unsigned char b0f1); void dilate0_erode1_4con(unsigned char *byt, size_t nr, size_t nc, unsigned char b0_f1); void dilate0_erode1_8con(unsigned char *byt, size_t nr, size_t nc, unsigned char b0_f1); void opening(unsigned char *byt, size_t s0, size_t s1, size_t depth, int con_type); void fillboundedholes(unsigned char *in, size_t s0, size_t s1, int anyblank); void maskbackorforeground(float *in, size_t size, unsigned char *byt, unsigned char b0f1); #endif gnuastro-0.2.33-8a3b/bin/noisechisel/binary.c0000644000175000017500000003760413001632540015626 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include "main.h" #include "label.h" #include "binary.h" /**************************************************************** ************** Binary NAN ***************** ****************************************************************/ /* When the float image has NaN pixels, set the respective byt value to GAL_FITS_BYTE_BLANK. */ void setbytblank(float *img, unsigned char *byt, size_t size) { float *end=img+size; do { if(isnan(*img++)) *byt=GAL_FITS_BYTE_BLANK; ++byt; } while(img=idx-2) /* Fill the full row if it is one of */ do *bp++=1; while(bp1 ? 1 : *n; while(++n Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef THRESH_H #define THRESH_H void findapplyqthreshold(struct noisechiselparams *p); void applydetectionthresholdskysub(struct noisechiselparams *p); void snthresh(struct noisechiselparams *p, float *sntable, size_t size, int det0seg1); #endif gnuastro-0.2.33-8a3b/bin/noisechisel/thresh.c0000644000175000017500000003035413001632540015632 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include "main.h" #include "binary.h" #include "noisechisel.h" /*********************************************************************/ /*************** Quantile threshold *********************/ /*********************************************************************/ void * qthreshonmesh(void *inparam) { struct gal_mesh_thread_params *mtp=(struct gal_mesh_thread_params *)inparam; struct gal_mesh_params *mp=mtp->mp; struct noisechiselparams *p=(struct noisechiselparams *)mp->params; float *mponeforall=mp->oneforall; float *oneforall=&mponeforall[mtp->id*mp->maxs0*mp->maxs1]; size_t modeindex=(size_t)(-1); size_t s0, s1, ind, row, num, start, is1=mp->s1; size_t i, *indexs=&mp->indexs[mtp->id*mp->thrdcols]; float *f, *img, *imgend, *inimg=p->conv, modesym=0.0f; float mirrordist=mp->mirrordist, minmodeq=mp->minmodeq; /* Start this thread's work: */ for(i=0;indexs[i]!=GAL_THREADS_NON_THRD_INDEX;++i) { /* Prepare the values: */ num=row=0; f=oneforall; ind=indexs[i]; start=mp->start[ind]; s0=mp->ts0[mp->types[ind]]; s1=mp->ts1[mp->types[ind]]; /* Copy all the non-NaN pixels images pixels of this mesh into the mesh array. Note that currently, the spatial positioning of the pixels is irrelevant, so we only keep those that are non-NaN.*/ do { imgend=(img = inimg + start + row++ * is1 ) + s1; do if(!isnan(*img)) { ++num; *f++ = *img; } while(++imgGAL_STATISTICS_MODE_SYM_GOOD && (float)modeindex/(float)num>minmodeq) { mp->garray1[ind] = oneforall[ gal_statistics_index_from_quantile(num, p->qthresh) ]; mp->garray2[ind] = oneforall[ gal_statistics_index_from_quantile(num, p->noerodequant) ]; } } } /* Free alltype and if multiple threads were used, wait until all other threads finish. */ if(mp->numthreads>1) pthread_barrier_wait(&mp->b); return NULL; } /* The threshold values are stored in the garray1 array of the gal_mesh_params structure. This function is basically identical to the gal_mesh_check_garray function in mesh.c, only in the middle, it does something else. See the comments there to better understand the process. */ void applythreshold(struct noisechiselparams *p) { struct gal_mesh_params *mp=&p->smp; /* `mp' instead of `smp' so you */ /* can try with p->lmp if you like. */ float qthreshv, nethreshv; unsigned char *b, *byt=p->byt; size_t gs0=mp->gs0, gs1=mp->gs1, nch1=mp->nch1; size_t s0, s1, fs1=mp->gs1*mp->nch1, chid, inchid; float *f, *fp, *garray1=mp->garray1, *array=p->conv; size_t *types=mp->types, *ts0=mp->ts0, *ts1=mp->ts1; size_t i, f0, f1, nmeshi=mp->nmeshi, nmeshc=mp->nmeshc; size_t row, startind, *start=mp->start, meshid, is1=mp->s1; /* Fill the array: */ for(i=0;ifgarray1) { f0=i/fs1; f1=i%fs1; inchid = (f0%gs0) * gs1 + f1%gs1; chid = (f0/gs0) * nch1 + f1/gs1; meshid = chid * nmeshc + inchid; } else meshid=i; /* Fill the output array with the value in this mesh: */ row=0; qthreshv=garray1[i]; s0=ts0[types[meshid]]; s1=ts1[types[meshid]]; startind=start[meshid]; nethreshv=mp->garray2[i]; do { b = byt + startind + row * is1; fp = ( f = array + startind + row * is1 ) + s1; do /* The image might have NaN pixels too, in which case any comparison will fail and the value in `b' will be 0, This is no problem, after this loop, all NaN pixels will be set to a fixed blank value. */ *b++ = ( *f>qthreshv ? ( *f>nethreshv ? BINARYNOOP : 1 ) : 0 ); while(++fanyblank) setbytblank(p->img, p->byt, p->smp.s0*p->smp.s1); } void findapplyqthreshold(struct noisechiselparams *p) { struct gal_mesh_params *mp=&p->smp; /* Find the threshold on each mesh that has the proper conditions. */ gal_mesh_operate_on_mesh(mp, qthreshonmesh, sizeof(float), 1, 1); if(p->threshname) gal_mesh_value_file(mp, p->threshname, "Quantile threshold value", "No erode threshold value", p->wcs, SPACK_STRING); /* Interpolate to have a value for each mesh. */ gal_mesh_interpolate(mp, "Interpolating quantile threshold"); if(p->threshname) gal_mesh_value_file(mp, p->threshname, "qthreshv interpolated", "nethreshv interpolated", p->wcs, SPACK_STRING); /* Smooth the interpolation */ gal_mesh_smooth(mp); if(p->threshname) gal_mesh_value_file(mp, p->threshname, "qthreshv smoothed", "nethreshv smoothed", p->wcs, SPACK_STRING); /* Apply the threshold on all the pixels: */ applythreshold(p); } /*********************************************************************/ /************** Average and STD threshold *******************/ /*********************************************************************/ /* This is very similar to the gal_mesh_check_garray function. The sky and its Standard deviation are stored in the garray1 and garray2 arrays of smp gal_mesh_params structure. */ void applydetectionthresholdskysub(struct noisechiselparams *p) { struct gal_mesh_params *smp=&p->smp; size_t is0=smp->s0; float *f, *in, sky, std; float dthresh=p->dthresh; unsigned char *b, *bf, *dbyt; size_t gid, row, start, chbasedid, *types=smp->types; size_t s0, s1, is1=smp->s1, *ts0=smp->ts0, *ts1=smp->ts1; /* Allocate the array to keep the threshold value: */ errno=0; dbyt=p->dbyt=malloc(is0*is1*sizeof *p->dbyt); if(dbyt==NULL) error(EXIT_FAILURE, errno, "%zu bytes for dbyt in " "applydetectionthreshold (detection.c)", is0*is1*sizeof *dbyt); /* Apply the threshold */ for(gid=0;gidnmeshi;++gid) { /* Get the meshid from i: */ chbasedid=gal_mesh_ch_based_id_from_gid(smp, gid); /* Fill the output array with the value in this mesh: */ row=0; sky = smp->garray1[gid]; std = smp->garray2[gid]; s0=ts0[types[chbasedid]]; s1=ts1[types[chbasedid]]; start=smp->start[chbasedid]; do { in = p->img + start + row*is1; f = p->imgss + start + row*is1; bf= ( b = dbyt + start + row++ * is1) + s1; do { /* The threshold is always very low. So for the majority of non-NaN pixels in the image, the condition above will be true. If we come over a NaN pixel, then by definition of NaN, all conditionals will fail. The benefit of this method of testing is that if an image doesn't have any NaN pixels, only the pixels below the threshold have to be checked for a NaN which are by definition a very small fraction of the total pixels. And if there are NaN pixels in the image, they will be checked. */ *b = ( (*f++=*in-sky) > dthresh*std ? 1 : isnan(*in) ? GAL_FITS_BYTE_BLANK : 0 ); ++in; } while(++bsegquant : p->detquant; char *name = det0seg1 ? "clumps" : "pseudo-detections"; char *histname= det0seg1 ? p->clumpsnhist : p->detectionsnhist; size_t snhistnbins= det0seg1 ? p->clumpsnhistnbins : p->detsnhistnbins; /* Check if the number is acceptable to the user. */ if(sizeminnumfalse) error(EXIT_FAILURE, 0, "there are only %zu %s in the sky region of " "the image. This is smaller than the minimum number you " "specified: %zu. You can decrease this minimum with the " "`--minnumfalse' (`-F') option or you can decrease the other " "parameters that determine the %s. See the GNU Astronomy " "Utilities manual (section on NoiseChisel) or Akhlaghi and " "Ichikawa (2015) for more information", size, name, p->minnumfalse, name); /* Sort the signal to noise ratios and remove their outliers */ qsort(sntable, size, sizeof *sntable, gal_qsort_float_increasing); /* The removal of outliers was useful when the S/N was calculated separately on each mesh (thus there were very few points). However, now that the S/N is calculated over the full image, the number of pseudo-detections and clumps is so high that these outliers will not play a significant role in the S/N threshold (unless you set unreasonably high quantiles!). So This is commented now. */ /*gal_statistics_remove_outliers_flat_cdf(sntable, &size);*/ /* Store the SN value. */ sn=sntable[gal_statistics_index_from_quantile(size, quant)]; if(p->cp.verb) { sprintf(report, "%s S/N: %.3f (%.3f quantile of %zu %s).", job, sn, quant, size, name); gal_timing_report(NULL, report, 2); } /* Put the S/N value in its proper place. */ if(det0seg1) p->clumpsn = sn; else p->detsn = sn; /* If the user has asked for it, make the histogram of the S/N distribution. */ if(snhistnbins) { /* For a check: if(ind!=0) continue; ff=(f=sntable)+numlabs; do printf("%f\n", *f++); while(frawtime), p->up.inputname, p->cp.hdu, size, name, quant, sn); gal_statistics_save_hist(sntable, size, snhistnbins, histname, cline); free(histname); } } gnuastro-0.2.33-8a3b/bin/noisechisel/noisechisel.h0000644000175000017500000000210712616616510016654 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef NOISECHISEL_H #define NOISECHISEL_H void noisechisel(struct noisechiselparams *p); #endif gnuastro-0.2.33-8a3b/bin/noisechisel/noisechisel.c0000644000175000017500000002425413001632540016644 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include "main.h" #include "sky.h" #include "label.h" #include "binary.h" #include "thresh.h" #include "detection.h" #include "noisechisel.h" #include "segmentation.h" /*********************************************************************/ /****************** NoiseChisel ***********************/ /*********************************************************************/ void makeoutput(struct noisechiselparams *p) { float *fpt; double *dpt; long num[0]; float *sky=NULL, *std=NULL; struct gal_fits_key_ll *keys=NULL; size_t s0=p->smp.s0, s1=p->smp.s1; /* First put a copy of the input image. */ gal_fits_array_to_file(p->cp.output, "Input", FLOAT_IMG, p->img, s0, s1, 0, p->wcs, NULL, SPACK_STRING); /* Add the necessary FITS keywords for MakeCatalog when reading the objects image. */ gal_fits_add_to_key_ll(&keys, TSTRING, "WCLUMPS", 0, "yes", 0, "Is there a clumps image companion?", 0, NULL); num[0]=p->numobjects-1; gal_fits_add_to_key_ll(&keys, TLONG, "NOBJS", 0, num, 0, "Number of objects in the image.", 0, NULL); dpt=&p->detsn; gal_fits_add_to_key_ll(&keys, TDOUBLE, "DETSN", 0, dpt, 0, "Signal to noise of true pseudo-detections.", 0, NULL); gal_fits_array_to_file(p->cp.output, "Objects", LONG_IMG, p->olab, s0, s1, p->anyblank, p->wcs, keys, SPACK_STRING); keys=NULL; /* keys was freed after writing. */ /* The clump labels, mentioning the total number of clumps. Note that even if no segmentation is to be done, we need this extension filled so the sky and its standard deviation can remain on the 3rd and 4th extensions. */ num[0] = p->detectonly ? 0 : p->numclumps-1; gal_fits_add_to_key_ll(&keys, TLONG, "NCLUMPS", 0, num, 0, "Number of clumps in the image.", 0, NULL); dpt=&p->clumpsn; gal_fits_add_to_key_ll(&keys, TDOUBLE, "CLUMPSN", 0, dpt, 0, "Signal to noise of true clumps.", 0, NULL); gal_fits_array_to_file(p->cp.output, "Clumps", LONG_IMG, p->clab, s0, s1, p->anyblank, p->wcs, keys, SPACK_STRING); keys=NULL; /* The sky image: */ gal_mesh_check_garray(&p->smp, &sky, &std); gal_fits_array_to_file(p->cp.output, "Sky", FLOAT_IMG, sky, s0, s1, 0, p->wcs, NULL, SPACK_STRING); /* The sky standard deviation image. Note that since this is a linked list, the median will be written to the FITS header first. Also note that these values were found before interpolating or smoothing the image, so we have put a "raw" in the comments of each variable.*/ fpt=&p->maxstd; gal_fits_add_to_key_ll(&keys, TFLOAT, "MAXSTD", 0, fpt, 0, "Maximum raw mesh sky standard deviation.", 0, NULL); fpt=&p->minstd; gal_fits_add_to_key_ll(&keys, TFLOAT, "MINSTD", 0, fpt, 0, "Minimum raw mesh sky standard deviation.", 0, NULL); fpt=&p->medstd; gal_fits_add_to_key_ll(&keys, TFLOAT, "MEDSTD", 0, fpt, 0, "Median raw mesh standard deviation.", 0, NULL); gal_fits_array_to_file(p->cp.output, "Standard deviation", FLOAT_IMG, std, s0, s1, 0, p->wcs, keys, SPACK_STRING); keys=NULL; /* Clean up: */ free(sky); free(std); } void noisechisel(struct noisechiselparams *p) { struct gal_mesh_params *smp=&p->smp, *lmp=&p->lmp; float *imgcopy; struct timeval t1; int verb=p->cp.verb; size_t i, s0=smp->s0, s1=smp->s1; char report[GAL_TIMING_VERB_MSG_LENGTH_V], *oreport; /* Convolve the image: */ if(verb) gettimeofday(&t1, NULL); gal_mesh_spatial_convolve_on_mesh(smp, &p->conv); if(p->detectionname) { gal_fits_array_to_file(p->detectionname, "Input", FLOAT_IMG, smp->img, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); gal_fits_array_to_file(p->detectionname, "Convolved", FLOAT_IMG, p->conv, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); } if(verb) gal_timing_report(&t1, "Convolved with kernel.", 1); /* Do the initial detection: */ if(verb) { gal_timing_report(NULL, "Starting to find initial detections.", 1); gettimeofday(&t1, NULL); } initialdetection(p); if(verb) { sprintf(report, "%zu initial detections found.", p->numobjects-1); gal_timing_report(&t1, report, 1); } /* Remove the false detections */ if(verb) { gal_timing_report(NULL, "Starting to find and remove false detections.", 1); gettimeofday(&t1, NULL); } onlytruedetections(p); if(verb) { sprintf(report, "%zu true detections identified.", p->numobjects-1); gal_timing_report(&t1, report, 1); } /* Dilate the byt array and find the new number of detections. Note that the connectivity has to be 8 connected. This is because we check the eight neighbors of every river pixel within each detection during the segmentation. Therefore if 4 connectivity is used here, two detection might be four connected and so their labels will be mixed during the checking of neighbors in the segmentation. */ if(verb) gettimeofday(&t1, NULL); if(p->dilate) { for(i=0;idilate;++i) dilate0_erode1_8con(p->byt, s0, s1, 0); p->numobjects=BF_concmp(p->byt, p->olab, s0, s1, p->anyblank, 8); if(verb) { sprintf(report, "%zu detections after %zu dilation%s", p->numobjects-1, p->dilate, p->dilate>1 ? "s." : "."); gal_timing_report(&t1, report, 1); } } if(p->detectionname) gal_fits_array_to_file(p->detectionname, "Dilated", LONG_IMG, p->olab, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); if(p->maskdetname) { gal_fits_array_to_file(p->maskdetname, "Input", FLOAT_IMG, p->img, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); gal_array_float_copy(p->img, s0*s1, &imgcopy); maskbackorforeground(imgcopy, s0*s1, p->byt, 0); gal_fits_array_to_file(p->maskdetname, "Undetected masked", FLOAT_IMG, imgcopy, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); free(imgcopy); gal_array_float_copy(p->img, s0*s1, &imgcopy); maskbackorforeground(imgcopy, s0*s1, p->byt, 1); gal_fits_array_to_file(p->maskdetname, "Detected masked", FLOAT_IMG, imgcopy, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); free(imgcopy); } /* Correct convolution if it was done on edges independently: */ if(smp->nch>1 && smp->fullconvolution==0 && p->detectonly==0) { if(verb) gettimeofday(&t1, NULL); gal_mesh_change_to_full_convolution(smp, p->conv); if(verb) gal_timing_report(&t1, "Convolved image internals corrected.", 1); } /* Find and subtract the final sky value for the input and convolved images. VERY IMPORTANT: ############### The sky value for the input image should be found after the convolved image. This is because findavestdongrid, will also set the p->cpscorr value and we want that from the input image, not the convolved image. */ if(verb) gettimeofday(&t1, NULL); if(p->detectonly==0) findsubtractskyconv(p); findavestdongrid(p, p->skyname); if(p->detectonly==0) subtractskyimg(p); if(verb) gal_timing_report(&t1, "Final sky and its STD found and subtracted.", 1); /* Segment the detections if segmentation is to be done. */ if(p->detectonly) clabwithnoseg(p->olab, p->clab, s0*s1, p->anyblank); else { if(verb) { gal_timing_report(NULL, "Starting to find clumps and objects.", 1); gettimeofday(&t1, NULL); } segmentation(p); if(verb) { sprintf(report, "%zu object%s""containing %zu clump%sfound.", p->numobjects-1, p->numobjects==2 ? " " : "s ", p->numclumps-1, p->numclumps ==2 ? " " : "s "); gal_timing_report(&t1, report, 1); } } /* Make the output: */ if(verb) gettimeofday(&t1, NULL); makeoutput(p); if(verb) { errno=0; oreport=malloc(strlen(p->cp.output)+100*sizeof *oreport); if(oreport==NULL) error(EXIT_FAILURE, errno, "%zu bytes for oreport in noisechisel " "(noisechisel.c)", strlen(p->cp.output)+100*sizeof *oreport); sprintf(oreport, "Output written to %s.", p->cp.output); gal_timing_report(&t1, oreport, 1); free(oreport); } /* Clean up: */ free(p->conv); /* Allocated in gal_mesh_spatial_convolve_on_mesh. */ gal_mesh_free_mesh(smp); /* Allocated here. */ gal_mesh_free_mesh(lmp); /* Allocated here. */ } gnuastro-0.2.33-8a3b/bin/noisechisel/args.h0000644000175000017500000004305112774161116015310 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef ARGS_H #define ARGS_H #include #include #include /**************************************************************/ /************** argp.h definitions ***************/ /**************************************************************/ /* Definition parameters for the argp: */ const char *argp_program_version=SPACK_STRING"\n"GAL_STRINGS_COPYRIGHT "\n\nWritten by Mohammad Akhlaghi"; const char *argp_program_bug_address=PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata"; const char doc[] = /* Before the list of options: */ GAL_STRINGS_TOP_HELP_INFO SPACK_NAME" Detects and segments signal that is deeply burried in noise. " "It employs a noise-based detection and segmentation method enabling it " "to be very resilient to the rich diversity of shapes in astronomical " "targets.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /* Available letters for short options: f j w x z A J K W X Y Z Used numbers: <=518 (except 515) Options with keys (second structure element) larger than 500 do not have a short version. */ static struct argp_option options[] = { { 0, 0, 0, 0, "Input:", 1 }, { "mask", 'M', "STR", 0, "Mask image file name.", 1 }, { "mhdu", 'H', "STR", 0, "Mask image header name.", 1 }, { "kernel", 'k', "STR", 0, "Kernel image file name.", 1 }, { "khdu", 'U', "STR", 0, "Kernel image header name.", 1 }, { "skysubtracted", 'E', 0, 0, "Input is already sky subtracted.", 1 }, { "minbfrac", 'B', "FLT", 0, "Minimum fraction of undetected area in a mesh.", 1 }, { "minnumfalse", 'F', "INT", 0, "Min No. of false detection/segments for quantile.", 1 }, { 0, 0, 0, 0, "Output:", 2 }, { "detectonly", 517, 0, 0, "Do not do any segmentation.", 2 }, { "grownclumps", 'C', 0, 0, "Save grownclumps instead of original clumps.", 2 }, { 0, 0, 0, 0, "Mesh grid:", 3 }, { "smeshsize", 's', "INT", 0, "Size of each small mesh (tile) in the grid.", 3 }, { "lmeshsize", 'l', "INT", 0, "Size of each large mesh (tile) in the grid.", 3 }, { "nch1", 'a', "INT", 0, "Number of channels along first FITS axis.", 3 }, { "nch2", 'b', "INT", 0, "Number of channels along second FITS axis.", 3 }, { "lastmeshfrac", 'L', "INT", 0, "Fraction of last mesh area to add new.", 3 }, { "mirrordist", 'd', "FLT", 0, "Distance beyond mirror point. Multiple of std.", 3 }, { "minmodeq", 'Q', "FLT", 0, "Minimum acceptable quantile for the mode.", 3 }, { "interponlyblank", 511, 0, 0, "Only interpolate over the blank pixels.", 3 }, { "numnearest", 'n', "INT", 0, "Number of nearest neighbors to interpolate.", 3 }, { "smoothwidth", 'T', "INT", 0, "Width of smoothing kernel (odd number).", 3 }, { "checkmesh", 500, 0, 0, "Store mesh IDs in `_mesh.fits' file.", 3 }, { "fullinterpolation", 501, 0, 0, "Ignore channels in interpolation.", 3 }, { "fullsmooth", 502, 0, 0, "Ignore channels in smoothing.", 3 }, { "fullconvolution", 504, 0, 0, "Ignore channels in convolution.", 3 }, { "meshbasedcheck", 516, 0, 0, "Each mesh in one pixel in mesh check images.", 3 }, { 0, 0, 0, 0, "Detection:", 4 }, { "qthresh", 't', "FLT", 0, "Quantile threshold on convolved image.", 4 }, { "erode", 'e', "INT", 0, "Num. erosions to apply after thresholding.", 4 }, { "erodengb", 506, "4or8", 0, "Use 4 or 8 connectivity in erosion.", 4 }, { "noerodequant", 503, "FLT", 0, "Quantile for no erosion.", 4 }, { "opening", 'p', "INT", 0, "Depth of opening to apply after erosion.", 4 }, { "openingngb", 507, "4or8", 0, "Use 4 or 8 connectivity in opening.", 4 }, { "sigclipmultip", 'u', "FLT", 0, "Multiple of standard deviation in sigma-clipping.", 4 }, { "sigcliptolerance", 'r', "FLT", 0, "Difference in STD tolerance to halt iteration.", 4 }, { "dthresh", 'R', "FLT", 0, "Threshold (STD multiple) for false detections.", 4 }, { "detsnminarea", 'i', "INT", 0, "Minimum area to calculate S/N in detection.", 4 }, { "detsnhistnbins", 510, "INT", 0, "Det. S/N histogram bins, suffix `_detsn.txt'.", 4 }, { "detquant", 'c', "FLT", 0, "False detections S/N quantile to find the true.", 4 }, { "dilate", 'I', "INT", 0, "Number of times to dilate true detections.", 4 }, { "checkthreshold", 505, 0, 0, "Threshold value on each mesh `_thresh.fits'.", 4 }, { "checkdetection", 508, 0, 0, "False detection steps in file `_det.fits'.", 4 }, { "checkdetectionsky", 509, 0, 0, "Sky for false detections in file `_detsky.fits'.", 4 }, { "checksky", 512, 0, 0, "Final sky and its STD per pixel `_sky.fits'.", 4 }, { "checkmaskdet", 518, 0, 0, "Mask detections and sky, `_maskdet.fits'.", 4 }, { 0, 0, 0, 0, "Segmentation:", 5 }, { "segsnminarea", 'm', "INT", 0, "Minimum area to find clumps S/N.", 5 }, { "segquant", 'g', "FLT", 0, "Signal to noise ratio quantile for clumps.", 5 }, { "clumpsnhistnbins", 514, "INT", 0, "Clump S/N histogram bins, suffix `_clumpsn.txt'.", 5 }, { "keepmaxnearriver", 'v', 0, 0, "Keep clumps with max touching river.", 5 }, { "gthresh", 'G', "FLT", 0, "Threshold (STD multiple) to stop growing clumps.", 5 }, { "minriverlength", 'y', 0, 0, "Minimum length of useful rivers in grown clumps.", 5 }, { "objbordersn", 'O', "FLT", 0, "Minimum S/N for grown clumps to be one object.", 5 }, { "checksegmentation", 513, 0, 0, "Store segmentation steps in file `_seg.fits'.", 5 }, { 0, 0, 0, 0, "Operating modes:", -1 }, {0} }; /* Parse a single option: */ static error_t parse_opt(int key, char *arg, struct argp_state *state) { /* Save the arguments structure: */ struct noisechiselparams *p = state->input; /* Set the pointer to the common parameters for all programs here: */ state->child_inputs[0]=&p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); switch(key) { /* Input: */ case 'M': gal_checkset_allocate_copy_set(arg, &p->up.maskname, &p->up.masknameset); break; case 'H': gal_checkset_allocate_copy_set(arg, &p->up.mhdu, &p->up.mhduset); break; case 'k': gal_checkset_allocate_copy_set(arg, &p->up.kernelname, &p->up.kernelnameset); break; case 'U': gal_checkset_allocate_copy_set(arg, &p->up.khdu, &p->up.khduset); break; case 'E': p->skysubtracted=1; p->up.skysubtractedset=1; break; case 'B': gal_checkset_float_l_0_s_1(arg, &p->minbfrac, "minbfrac", key, SPACK, NULL, 0); p->up.minbfracset=1; break; case 'F': gal_checkset_sizet_l_zero(arg, &p->minnumfalse, "minnumfalse", key, SPACK, NULL, 0); p->up.minnumfalseset=1; break; /* Output: */ case 517: p->detectonly=1; break; case 'C': p->grownclumps=1; p->up.grownclumpsset=1; break; /* Mesh grid: */ case 's': gal_checkset_sizet_l_zero(arg, &p->smp.meshsize, "smeshsize", key, SPACK, NULL, 0); p->up.smeshsizeset=1; break; case 'l': gal_checkset_sizet_l_zero(arg, &p->lmp.meshsize, "lmeshsize", key, SPACK, NULL, 0); p->up.lmeshsizeset=1; break; case 'a': gal_checkset_sizet_l_zero(arg, &p->smp.nch1, "nch1", key, SPACK, NULL, 0); p->up.nch1set=1; break; case 'b': gal_checkset_sizet_l_zero(arg, &p->smp.nch2, "nch2", key, SPACK, NULL, 0); p->up.nch2set=1; break; case 'L': gal_checkset_float_l_0_s_1(arg, &p->smp.lastmeshfrac, "lastmeshfrac", key, SPACK, NULL, 0); p->up.lastmeshfracset=1; break; case 'd': gal_checkset_float_l_0(arg, &p->smp.mirrordist, "mirrordist", key, SPACK, NULL, 0); p->up.mirrordistset=1; break; case 'Q': gal_checkset_float_l_0_s_1(arg, &p->smp.minmodeq, "minmodeq", key, SPACK, NULL, 0); p->up.minmodeqset=1; break; case 511: p->smp.interponlyblank=1; break; case 'n': gal_checkset_sizet_l_zero(arg, &p->smp.numnearest, "numnearest", key, SPACK, NULL, 0); p->up.numnearestset=1; break; case 'T': gal_checkset_sizet_p_odd(arg, &p->smp.smoothwidth, "smoothwidth", key, SPACK, NULL, 0); p->up.smoothwidthset=1; break; case 500: p->meshname="a"; /* Just a placeholder! It will be corrected later */ break; case 501: p->smp.fullinterpolation=1; p->up.fullinterpolationset=1; break; case 502: p->smp.fullsmooth=1; p->up.fullsmoothset=1; break; case 504: p->smp.fullconvolution=1; p->up.fullconvolutionset=1; break; case 516: p->smp.meshbasedcheck=1; break; /* Detection */ case 't': gal_checkset_float_l_0_s_1(arg, &p->qthresh, "qthresh", key, SPACK, NULL, 0); p->up.qthreshset=1; break; case 'e': gal_checkset_sizet_el_zero(arg, &p->erode, "erode", key, SPACK, NULL, 0); p->up.erodeset=1; break; case 506: gal_checkset_int_4_or_8(arg, &p->erodengb, "erodengb", key, SPACK, NULL, 0); p->up.erodengbset=1; break; case 503: gal_checkset_float_l_0_s_1(arg, &p->noerodequant, "noerodequant", key, SPACK, NULL, 0); p->up.noerodequantset=1; break; case 'p': gal_checkset_sizet_el_zero(arg, &p->opening, "opening", key, SPACK, NULL, 0); p->up.openingset=1; break; case 507: gal_checkset_int_4_or_8(arg, &p->openingngb, "openingngb", key, SPACK, NULL, 0); p->up.openingngbset=1; break; case 'u': gal_checkset_float_l_0(arg, &p->sigclipmultip, "sigclipmultip", key, SPACK, NULL, 0); p->up.sigclipmultipset=1; break; case 'r': gal_checkset_float_l_0_s_1(arg, &p->sigcliptolerance, "sigcliptolerance", key, SPACK, NULL, 0); p->up.sigcliptoleranceset=1; break; case 'R': gal_checkset_any_float(arg, &p->dthresh, "dthresh", key, SPACK, NULL, 0); p->up.dthreshset=1; break; case 'i': gal_checkset_sizet_l_zero(arg, &p->detsnminarea, "detsnminarea", key, SPACK, NULL, 0); p->up.detsnminareaset=1; break; case 510: gal_checkset_sizet_el_zero(arg, &p->detsnhistnbins, "detsnhistnbins", key, SPACK, NULL, 0); p->up.detsnhistnbinsset=1; break; case 'c': gal_checkset_float_l_0_s_1(arg, &p->detquant, "detquant", key, SPACK, NULL, 0); p->up.detquantset=1; break; case 'I': gal_checkset_sizet_el_zero(arg, &p->dilate, "dilate", key, SPACK, NULL, 0); p->up.dilateset=1; break; case 505: p->threshname="a"; break; case 508: p->detectionname="a"; break; case 509: p->detectionskyname="a"; break; case 512: p->skyname="a"; break; case 518: p->maskdetname="a"; break; /* Segmentation: */ case 'm': gal_checkset_sizet_l_zero(arg, &p->segsnminarea, "segsnminarea", key, SPACK, NULL, 0); p->up.segsnminareaset=1; break; case 'g': gal_checkset_float_l_0_s_1(arg, &p->segquant, "segquant", key, SPACK, NULL, 0); p->up.segquantset=1; break; case 'v': p->keepmaxnearriver=1; break; case 'G': gal_checkset_any_float(arg, &p->gthresh, "gthresh", key, SPACK, NULL, 0); p->up.gthreshset=1; break; case 'y': gal_checkset_sizet_l_zero(arg, &p->minriverlength, "minriverlength", key, SPACK, NULL, 0); p->up.minriverlengthset=1; break; case 'O': gal_checkset_float_l_0(arg, &p->objbordersn, "objbordersn", key, SPACK, NULL, 0); p->up.objbordersnset=1; break; case 514: gal_checkset_sizet_el_zero(arg, &p->clumpsnhistnbins, "clumpsnhistnbins", key, SPACK, NULL, 0); p->up.clumpsnhistnbinsset=1; break; case 513: p->segmentationname="a"; break; /* Operating modes: */ /* Read the non-option arguments: */ case ARGP_KEY_ARG: /* See what type of input value it is and put it in. */ if( gal_fits_name_is_fits(arg) ) { if(p->up.inputname) argp_error(state, "only one input image should be given"); else p->up.inputname=arg; } else argp_error(state, "%s is not a valid file type", arg); break; /* The command line options and arguments are finished. */ case ARGP_KEY_END: if(p->cp.setdirconf==0 && p->cp.setusrconf==0 && p->cp.printparams==0) { if(state->arg_num==0) argp_error(state, "no argument given"); if(p->up.inputname==NULL) argp_error(state, "no input FITS image(s) provided"); } break; default: return ARGP_ERR_UNKNOWN; } return 0; } /* Specify the children parsers: */ struct argp_child children[]= { {&commonargp, 0, NULL, 0}, {0, 0, 0, 0} }; /* Basic structure defining the whole argument reading process. */ static struct argp thisargp = {options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif gnuastro-0.2.33-8a3b/bin/noisechisel/ui.h0000644000175000017500000000223512616616510014766 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef IMCROPUI_H #define IMCROPUI_H void setparams(int argc, char *argv[], struct noisechiselparams *p); void freeandreport(struct noisechiselparams *p, struct timeval *t1); #endif gnuastro-0.2.33-8a3b/bin/noisechisel/ui.c0000644000175000017500000011051013001632540014743 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include /* From Gnulib. */ #include /* includes time.h and sys/time.h */ #include #include #include #include "main.h" #include "ui.h" /* Needs main.h */ #include "args.h" /* Needs main.h, includes argp.h. */ /* Set the file names of the places where the default parameters are put. */ #define CONFIG_FILE SPACK CONF_POSTFIX #define SYSCONFIG_FILE SYSCONFIG_DIR "/" CONFIG_FILE #define USERCONFIG_FILEEND USERCONFIG_DIR CONFIG_FILE #define CURDIRCONFIG_FILE CURDIRCONFIG_DIR CONFIG_FILE /**************************************************************/ /************** Options and parameters ***************/ /**************************************************************/ void readconfig(char *filename, struct noisechiselparams *p) { FILE *fp; size_t lineno=0, len=200; char *line, *name, *value; struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; char key='a'; /* Not used, just a place holder. */ /* When the file doesn't exist or can't be opened, it is ignored. It might be intentional, so there is no error. If a parameter is missing, it will be reported after all defaults are read. */ fp=fopen(filename, "r"); if (fp==NULL) return; /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); /* Read the tokens in the file: */ while(getline(&line, &len, fp) != -1) { /* Prepare the "name" and "value" strings, also set lineno. */ GAL_CONFIGFILES_START_READING_LINE; /* Inputs: */ if(strcmp(name, "hdu")==0) gal_checkset_allocate_copy_set(value, &cp->hdu, &cp->hduset); else if(strcmp(name, "mask")==0) gal_checkset_allocate_copy_set(value, &up->maskname, &up->masknameset); else if(strcmp(name, "mhdu")==0) gal_checkset_allocate_copy_set(value, &up->mhdu, &up->mhduset); else if(strcmp(name, "kernel")==0) gal_checkset_allocate_copy_set(value, &up->kernelname, &up->kernelnameset); else if(strcmp(name, "khdu")==0) gal_checkset_allocate_copy_set(value, &up->khdu, &up->khduset); else if(strcmp(name, "skysubtracted")==0) { if(up->skysubtractedset) continue; gal_checkset_int_zero_or_one(value, &p->skysubtracted, name, key, SPACK, filename, lineno); up->skysubtractedset=1; } else if(strcmp(name, "minbfrac")==0) { if(up->minbfracset) continue; gal_checkset_float_l_0_s_1(value, &p->minbfrac, name, key, SPACK, filename, lineno); up->minbfracset=1; } else if(strcmp(name, "minnumfalse")==0) { if(up->minnumfalseset) continue; gal_checkset_sizet_l_zero(value, &p->minnumfalse, name, key, SPACK, filename, lineno); up->minnumfalseset=1; } /* Outputs */ else if(strcmp(name, "output")==0) gal_checkset_allocate_copy_set(value, &cp->output, &cp->outputset); else if(strcmp(name, "grownclumps")==0) { if(up->grownclumpsset) continue; gal_checkset_int_zero_or_one(value, &p->grownclumps, name, key, SPACK, filename, lineno); up->grownclumpsset=1; } /* Mesh grid: */ else if(strcmp(name, "smeshsize")==0) { if(up->smeshsizeset) continue; gal_checkset_sizet_l_zero(value, &p->smp.meshsize, name, key, SPACK, filename, lineno); up->smeshsizeset=1; } else if(strcmp(name, "lmeshsize")==0) { if(up->lmeshsizeset) continue; gal_checkset_sizet_l_zero(value, &p->lmp.meshsize, name, key, SPACK, filename, lineno); up->lmeshsizeset=1; } else if(strcmp(name, "nch1")==0) { if(up->nch1set) continue; gal_checkset_sizet_l_zero(value, &p->smp.nch1, name, key, SPACK, filename, lineno); up->nch1set=1; } else if(strcmp(name, "nch2")==0) { if(up->nch2set) continue; gal_checkset_sizet_l_zero(value, &p->smp.nch2, name, key, SPACK, filename, lineno); up->nch2set=1; } else if(strcmp(name, "lastmeshfrac")==0) { if(up->lastmeshfracset) continue; gal_checkset_float_l_0_s_1(value, &p->smp.lastmeshfrac, name, key, SPACK, filename, lineno); up->lastmeshfracset=1; } else if(strcmp(name, "mirrordist")==0) { if(up->mirrordistset) continue; gal_checkset_float_l_0(value, &p->smp.mirrordist, name, key, SPACK, filename, lineno); up->mirrordistset=1; } else if(strcmp(name, "minmodeq")==0) { if(up->minmodeqset) continue; gal_checkset_float_l_0_s_1(value, &p->smp.minmodeq, name, key, SPACK, filename, lineno); up->minmodeqset=1; } else if(strcmp(name, "numnearest")==0) { if(up->numnearestset) continue; gal_checkset_sizet_l_zero(value, &p->smp.numnearest, name, key, SPACK, filename, lineno); up->numnearestset=1; } else if(strcmp(name, "smoothwidth")==0) { if(up->smoothwidthset) continue; gal_checkset_sizet_p_odd(value, &p->smp.smoothwidth, name, key, SPACK, filename, lineno); up->smoothwidthset=1; } else if(strcmp(name, "fullconvolution")==0) { if(up->fullconvolutionset) continue; gal_checkset_int_zero_or_one(value, &p->smp.fullconvolution, name, key, SPACK, filename, lineno); up->fullconvolutionset=1; } else if(strcmp(name, "fullinterpolation")==0) { if(up->fullinterpolationset) continue; gal_checkset_int_zero_or_one(value, &p->smp.fullinterpolation, name, key, SPACK, filename, lineno); up->fullinterpolationset=1; } else if(strcmp(name, "fullsmooth")==0) { if(up->fullsmoothset) continue; gal_checkset_int_zero_or_one(value, &p->smp.fullsmooth, name, key, SPACK, filename, lineno); up->fullsmoothset=1; } /* Detection: */ else if(strcmp(name, "qthresh")==0) { if(up->qthreshset) continue; gal_checkset_float_l_0_s_1(value, &p->qthresh, name, key, SPACK, filename, lineno); up->qthreshset=1; } else if(strcmp(name, "erode")==0) { if(up->erodeset) continue; gal_checkset_sizet_el_zero(value, &p->erode, name, key, SPACK, filename, lineno); up->erodeset=1; } else if(strcmp(name, "erodengb")==0) { if(up->erodengbset) continue; gal_checkset_int_4_or_8(value, &p->erodengb, name, key, SPACK, filename, lineno); up->erodengbset=1; } else if(strcmp(name, "noerodequant")==0) { if(up->noerodequantset) continue; gal_checkset_float_l_0_s_1(value, &p->noerodequant, name, key, SPACK, filename, lineno); up->noerodequantset=1; } else if(strcmp(name, "opening")==0) { if(up->openingset) continue; gal_checkset_sizet_el_zero(value, &p->opening, name, key, SPACK, filename, lineno); up->openingset=1; } else if(strcmp(name, "openingngb")==0) { if(up->openingngbset) continue; gal_checkset_int_4_or_8(value, &p->openingngb, name, key, SPACK, filename, lineno); up->openingngbset=1; } else if(strcmp(name, "sigclipmultip")==0) { if(up->sigclipmultipset) continue; gal_checkset_float_l_0(value, &p->sigclipmultip, name, key, SPACK, filename, lineno); up->sigclipmultipset=1; } else if(strcmp(name, "sigcliptolerance")==0) { if(up->sigcliptoleranceset) continue; gal_checkset_float_l_0_s_1(value, &p->sigcliptolerance, name, key, SPACK, filename, lineno); up->sigcliptoleranceset=1; } else if(strcmp(name, "dthresh")==0) { if(up->dthreshset) continue; gal_checkset_any_float(value, &p->dthresh, name, key, SPACK, filename, lineno); up->dthreshset=1; } else if(strcmp(name, "detsnminarea")==0) { if(up->detsnminareaset) continue; gal_checkset_sizet_l_zero(value, &p->detsnminarea, name, key, SPACK, filename, lineno); up->detsnminareaset=1; } else if(strcmp(name, "detsnhistnbins")==0) { if(up->detsnhistnbinsset) continue; gal_checkset_sizet_el_zero(value, &p->detsnhistnbins, name, key, SPACK, filename, lineno); up->detsnhistnbinsset=1; } else if(strcmp(name, "detquant")==0) { if(up->detquantset) continue; gal_checkset_float_l_0_s_1(value, &p->detquant, name, key, SPACK, filename, lineno); up->detquantset=1; } else if(strcmp(name, "dilate")==0) { if(up->dilateset) continue; gal_checkset_sizet_el_zero(value, &p->dilate, name, key, SPACK, filename, lineno); up->dilateset=1; } /* Segmentation: */ else if(strcmp(name, "segsnminarea")==0) { if(up->segsnminareaset) continue; gal_checkset_sizet_l_zero(value, &p->segsnminarea, name, key, SPACK, filename, lineno); up->segsnminareaset=1; } else if(strcmp(name, "keepmaxnearriver")==0) { if(up->keepmaxnearriverset) continue; gal_checkset_int_zero_or_one(value, &p->keepmaxnearriver, name, key, SPACK, filename, lineno); up->keepmaxnearriverset=1; } else if(strcmp(name, "segquant")==0) { if(up->segquantset) continue; gal_checkset_float_l_0_s_1(value, &p->segquant, name, key, SPACK, filename, lineno); up->segquantset=1; } else if(strcmp(name, "clumpsnhistnbins")==0) { if(up->clumpsnhistnbinsset) continue; gal_checkset_sizet_el_zero(value, &p->clumpsnhistnbins, name, key, SPACK,filename, lineno); up->clumpsnhistnbinsset=1; } else if(strcmp(name, "gthresh")==0) { if(up->gthreshset) continue; gal_checkset_any_float(value, &p->gthresh, name, key, SPACK, filename, lineno); up->gthreshset=1; } else if(strcmp(name, "minriverlength")==0) { if(up->minriverlengthset) continue; gal_checkset_sizet_l_zero(value, &p->minriverlength, name, key, SPACK, filename, lineno); up->minriverlengthset=1; } else if(strcmp(name, "objbordersn")==0) { if(up->objbordersnset) continue; gal_checkset_float_l_0(value, &p->objbordersn, name, key, SPACK, filename, lineno); up->objbordersnset=1; } /* Operating modes: */ /* Read options common to all programs */ GAL_CONFIGFILES_READ_COMMONOPTIONS_FROM_CONF else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s` not recognized.\n", name); } free(line); fclose(fp); } void printvalues(FILE *fp, struct noisechiselparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; struct gal_mesh_params *smp=&p->smp, *lmp=&p->lmp; /* Print all the options that are set. Separate each group with a commented line explaining the options in that group. */ fprintf(fp, "\n# Input:\n"); if(cp->hduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("hdu", cp->hdu); if(up->masknameset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("mask", up->maskname); if(up->mhdu) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("mhdu", up->mhdu); if(up->kernelnameset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("kernel", up->kernelname); if(up->khdu) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("khdu", up->khdu); if(up->skysubtractedset) fprintf(fp, CONF_SHOWFMT"%d\n", "skysubtracted", p->skysubtracted); if(up->minbfracset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "minbfrac", p->minbfrac); if(up->minnumfalseset) fprintf(fp, CONF_SHOWFMT"%zu\n", "minnumfalse", p->minnumfalse); fprintf(fp, "\n# Output:\n"); if(cp->outputset) fprintf(fp, CONF_SHOWFMT"%s\n", "output", cp->output); if(up->grownclumpsset) fprintf(fp, CONF_SHOWFMT"%d\n", "grownclumps", p->grownclumps); fprintf(fp, "\n# Mesh grid:\n"); if(up->smeshsizeset) fprintf(fp, CONF_SHOWFMT"%zu\n", "smeshsize", smp->meshsize); if(up->lmeshsizeset) fprintf(fp, CONF_SHOWFMT"%zu\n", "lmeshsize", lmp->meshsize); if(up->nch1set) fprintf(fp, CONF_SHOWFMT"%zu\n", "nch1", smp->nch1); if(up->nch2set) fprintf(fp, CONF_SHOWFMT"%zu\n", "nch2", smp->nch2); if(up->lastmeshfracset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "lastmeshfrac", smp->lastmeshfrac); if(up->mirrordistset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "mirrordist", smp->mirrordist); if(up->minmodeqset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "minmodeq", smp->minmodeq); if(up->numnearestset) fprintf(fp, CONF_SHOWFMT"%zu\n", "numnearest", smp->numnearest); if(up->smoothwidthset) fprintf(fp, CONF_SHOWFMT"%zu\n", "smoothwidth", smp->smoothwidth); if(up->fullconvolutionset) fprintf(fp, CONF_SHOWFMT"%d\n", "fullconvolution", smp->fullconvolution); if(up->fullinterpolationset) fprintf(fp, CONF_SHOWFMT"%d\n", "fullinterpolation", smp->fullinterpolation); if(up->fullsmoothset) fprintf(fp, CONF_SHOWFMT"%d\n", "fullsmooth", smp->fullsmooth); fprintf(fp, "\n# Detection:\n"); if(up->qthreshset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "qthresh", p->qthresh); if(up->erodeset) fprintf(fp, CONF_SHOWFMT"%zu\n", "erode", p->erode); if(up->erodengbset) fprintf(fp, CONF_SHOWFMT"%d\n", "erodengb", p->erodengb); if(up->noerodequantset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "noerodequant", p->noerodequant); if(up->openingset) fprintf(fp, CONF_SHOWFMT"%zu\n", "opening", p->opening); if(up->openingngbset) fprintf(fp, CONF_SHOWFMT"%d\n", "openingngb", p->openingngb); if(up->sigclipmultipset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "sigclipmultip", p->sigclipmultip); if(up->sigcliptoleranceset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "sigcliptolerance", p->sigcliptolerance); if(up->dthreshset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "dthresh", p->dthresh); if(up->detsnminareaset) fprintf(fp, CONF_SHOWFMT"%zu\n", "detsnminarea", p->detsnminarea); if(up->detsnhistnbinsset) fprintf(fp, CONF_SHOWFMT"%zu\n", "detsnhistnbins", p->detsnhistnbins); if(up->detquantset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "detquant", p->detquant); if(up->dilateset) fprintf(fp, CONF_SHOWFMT"%zu\n", "dilate", p->dilate); fprintf(fp, "\n# Segmentation:\n"); if(up->segsnminareaset) fprintf(fp, CONF_SHOWFMT"%zu\n", "segsnminarea", p->segsnminarea); if(up->keepmaxnearriverset) fprintf(fp, CONF_SHOWFMT"%d\n", "keepmaxnearriver", p->keepmaxnearriver); if(up->segquantset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "segquant", p->segquant); if(up->clumpsnhistnbinsset) fprintf(fp, CONF_SHOWFMT"%zu\n", "clumpsnhistnbins", p->clumpsnhistnbins); if(up->gthreshset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "gthresh", p->gthresh); if(up->minriverlengthset) fprintf(fp, CONF_SHOWFMT"%zu\n", "minriverlength", p->minriverlength); if(up->objbordersnset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "objbordersn", p->objbordersn); /* For the operating mode, first put the macro to print the common options, then the (possible options particular to this program). */ fprintf(fp, "\n# Operating mode:\n"); GAL_CONFIGFILES_PRINT_COMMONOPTIONS; } /* Note that numthreads will be used automatically based on the configure time. */ void checkifset(struct noisechiselparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; int intro=0; if(cp->hduset==0) GAL_CONFIGFILES_REPORT_NOTSET("hdu"); if(up->khduset==0) GAL_CONFIGFILES_REPORT_NOTSET("khdu"); if(up->skysubtractedset==0) GAL_CONFIGFILES_REPORT_NOTSET("skysubtracted"); if(up->minbfracset==0) GAL_CONFIGFILES_REPORT_NOTSET("minbfrac"); if(up->minnumfalseset==0) GAL_CONFIGFILES_REPORT_NOTSET("minnumfalse"); /* Output */ if(up->grownclumpsset==0) GAL_CONFIGFILES_REPORT_NOTSET("grownclumps"); /* Mesh grid: */ if(up->smeshsizeset==0) GAL_CONFIGFILES_REPORT_NOTSET("smeshsize"); if(up->lmeshsizeset==0) GAL_CONFIGFILES_REPORT_NOTSET("lmeshsize"); if(up->nch1set==0) GAL_CONFIGFILES_REPORT_NOTSET("nch1"); if(up->nch2set==0) GAL_CONFIGFILES_REPORT_NOTSET("nch2"); if(up->lastmeshfracset==0) GAL_CONFIGFILES_REPORT_NOTSET("lastmeshfrac"); if(up->mirrordistset==0) GAL_CONFIGFILES_REPORT_NOTSET("mirrordist"); if(up->minmodeqset==0) GAL_CONFIGFILES_REPORT_NOTSET("minmodeq"); if(up->numnearestset==0) GAL_CONFIGFILES_REPORT_NOTSET("numnearest"); if(up->smoothwidthset==0) GAL_CONFIGFILES_REPORT_NOTSET("smoothwidth"); if(up->fullconvolutionset==0) GAL_CONFIGFILES_REPORT_NOTSET("fullconvolution"); if(up->fullinterpolationset==0) GAL_CONFIGFILES_REPORT_NOTSET("fullinterpolation"); if(up->fullsmoothset==0) GAL_CONFIGFILES_REPORT_NOTSET("fullsmooth"); /* Detection: */ if(up->qthreshset==0) GAL_CONFIGFILES_REPORT_NOTSET("qthresh"); if(up->erodeset==0) GAL_CONFIGFILES_REPORT_NOTSET("erode"); if(up->erodengbset==0) GAL_CONFIGFILES_REPORT_NOTSET("erodengb"); if(up->noerodequantset==0) GAL_CONFIGFILES_REPORT_NOTSET("noerodequant"); if(up->openingset==0) GAL_CONFIGFILES_REPORT_NOTSET("opening"); if(up->openingngbset==0) GAL_CONFIGFILES_REPORT_NOTSET("openingngb"); if(up->sigclipmultipset==0) GAL_CONFIGFILES_REPORT_NOTSET("sigclipmultip"); if(up->sigcliptoleranceset==0) GAL_CONFIGFILES_REPORT_NOTSET("sigcliptolerance"); if(up->dthreshset==0) GAL_CONFIGFILES_REPORT_NOTSET("dthresh"); if(up->detsnminareaset==0) GAL_CONFIGFILES_REPORT_NOTSET("detsnminarea"); if(up->detsnhistnbinsset==0) GAL_CONFIGFILES_REPORT_NOTSET("detsnhistnbins"); if(up->detquantset==0) GAL_CONFIGFILES_REPORT_NOTSET("detquant"); if(up->dilateset==0) GAL_CONFIGFILES_REPORT_NOTSET("dilate"); /* Segmentation: */ if(up->segsnminareaset==0) GAL_CONFIGFILES_REPORT_NOTSET("segsnminarea"); if(up->keepmaxnearriverset==0) GAL_CONFIGFILES_REPORT_NOTSET("keepmaxnearriver"); if(up->segquantset==0) GAL_CONFIGFILES_REPORT_NOTSET("segquant"); if(up->clumpsnhistnbinsset==0) GAL_CONFIGFILES_REPORT_NOTSET("clumpsnhistnbins"); if(up->gthreshset==0) GAL_CONFIGFILES_REPORT_NOTSET("gthresh"); if(up->minriverlengthset==0) GAL_CONFIGFILES_REPORT_NOTSET("minriverlength"); if(up->objbordersnset==0) GAL_CONFIGFILES_REPORT_NOTSET("objbordersn"); GAL_CONFIGFILES_END_OF_NOTSET_REPORT; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ void sanitycheck(struct noisechiselparams *p) { struct gal_mesh_params *smp=&p->smp; /* Make sure the input file exists. */ gal_checkset_check_file(p->up.inputname); /* Make sure that the noerode quantile is larger than qthresh. */ if( p->noerodequant <= p->qthresh) error(EXIT_FAILURE, 0, "The quantile for no erosion (`--noerodequant') " "must be larger than the base quantile threshold (`--qthresh', " "or `-t'). You have provided %.4f and %.4f for the former and " "latter, respectively.", p->noerodequant, p->qthresh); /* Set the maskname and mask hdu accordingly: */ gal_fits_file_or_ext_name(p->up.inputname, p->cp.hdu, p->up.masknameset, &p->up.maskname, p->up.mhdu, p->up.mhduset, "mask"); /* Set the output name: */ if(p->cp.output) { gal_checkset_check_remove_file(p->cp.output, p->cp.dontdelete); /* When the output name is given (possibly with directory information), the user certainly wants the directory information, if they have bothered to include it. */ p->cp.removedirinfo=0; } else gal_checkset_automatic_output(p->up.inputname, "_labeled.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->cp.output); /* Set the check image names: */ if(p->meshname) { p->meshname=NULL; /* Was not allocated before! */ gal_checkset_automatic_output(p->cp.output, "_meshs.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->meshname); } if(p->threshname) { p->threshname=NULL; gal_checkset_automatic_output(p->cp.output, "_thresh.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->threshname); } if(p->detectionname) { p->detectionname=NULL; gal_checkset_automatic_output(p->cp.output, "_det.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->detectionname); } if(p->detectionskyname) { p->detectionskyname=NULL; gal_checkset_automatic_output(p->cp.output, "_detsky.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->detectionskyname); } if(p->detsnhistnbins) { p->detectionsnhist=NULL; gal_checkset_automatic_output(p->cp.output, "_detsn.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->detectionsnhist); } if(p->skyname) { p->skyname=NULL; gal_checkset_automatic_output(p->cp.output, "_sky.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->skyname); } if(p->segmentationname) { p->segmentationname=NULL; gal_checkset_automatic_output(p->cp.output, "_seg.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->segmentationname); } if(p->clumpsnhistnbins) { p->clumpsnhist=NULL; gal_checkset_automatic_output(p->cp.output, "_clumpsn.txt", p->cp.removedirinfo, p->cp.dontdelete, &p->clumpsnhist); } if(p->maskdetname) { p->maskdetname=NULL; gal_checkset_automatic_output(p->cp.output, "_maskdet.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->maskdetname); } /* Other checks: */ if(smp->numnearestnumnearest); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ /* The default PSF. It was created by saving the following commands in a script and running it. The crop is because the first and last rows of all PSFs made by MakeProfiles is blank (zero). You can keep the spaces when copying and pasting ;-). Just make it executable and run it. set -o errexit # Stop if a program returns false. echo "0 0.0 0.0 2 2 0 0 1 1 5" > tmp.txt export GSL_RNG_TYPE=ranlxs2 export GSL_RNG_SEED=1 astmkprof tmp.txt --oversample=1 --envseed --numrandom=10000 \ --tolerance=0.01 astimgcrop 0.fits --section=2:*,2:* --zeroisnotblank --output=fwhm2.fits astconvertt fwhm2.fits --output=fwhm2.txt rm 0.fits tmp.fits *.log tmp.txt */ size_t defaultkernel_s0=11; size_t defaultkernel_s1=11; float defaultkernel[121]= { 0, 0, 0, 0, 0, 2.58073e-08, 0, 0, 0, 0, 0, 0, 0, 2.90237e-08, 6.79851e-07, 4.4435e-06, 8.31499e-06, 4.50166e-06, 6.97185e-07, 3.00904e-08, 0, 0, 0, 2.87873e-08, 2.48435e-06, 5.81339e-05, 0.000379508, 0.000709334, 0.000383714, 5.94125e-05, 2.56498e-06, 3.00032e-08, 0, 0, 6.70501e-07, 5.77826e-05, 0.00134992, 0.00879665, 0.0164126, 0.00886609, 0.00137174, 5.92134e-05, 6.92853e-07, 0, 0, 4.3798e-06, 0.000376616, 0.00877689, 0.0570404, 0.106142, 0.0572108, 0.00883846, 0.000381257, 4.46059e-06, 0, 2.54661e-08, 8.24845e-06, 0.00070725, 0.0164287, 0.10639, 0.19727, 0.106003, 0.0163402, 0.000703951, 8.23152e-06, 2.55057e-08, 0, 4.5229e-06, 0.000386632, 0.00894947, 0.0577282, 0.106614, 0.0570877, 0.00877699, 0.000377496, 4.41036e-06, 0, 0, 7.1169e-07, 6.0678e-05, 0.00140013, 0.00899917, 0.0165582, 0.00883658, 0.00135509, 5.81823e-05, 6.79067e-07, 0, 0, 3.12002e-08, 2.65502e-06, 6.11192e-05, 0.000391739, 0.000718637, 0.000382453, 5.85194e-05, 2.50864e-06, 2.9249e-08, 0, 0, 0, 3.14197e-08, 7.22146e-07, 4.61954e-06, 8.45613e-06, 4.49082e-06, 6.85919e-07, 2.9364e-08, 0, 0, 0, 0, 0, 0, 0, 2.63305e-08, 0, 0, 0, 0, 0 }; void preparearrays(struct noisechiselparams *p) { struct gal_mesh_params *smp=&p->smp, *lmp=&p->lmp; long *meshindexs; float *f, *ff, *fp; size_t *relngb=p->relngb, s0, s1; /* Read the input image in. Note that the pointer to the image is also kept in p->img. Since some of the mesh operations should be done on the convolved image and some on the actual image, we will need to change the mesh's img value some times and the p->img will be used to keep its actual value. */ gal_fits_file_to_float(p->up.inputname, p->up.maskname, p->cp.hdu, p->up.mhdu, (float **)&smp->img, &p->bitpix, &p->anyblank, &smp->s0, &smp->s1); gal_fits_read_wcs(p->up.inputname, p->cp.hdu, 0, 0, &p->nwcs, &p->wcs); s0=smp->s0; s1=smp->s1; /* make sure the channel sizes fit the channel sizes. */ if( s0%smp->nch2 || s1%smp->nch1 ) error(EXIT_FAILURE, 0, "the input image size (%zu x %zu) is not an " "exact multiple of the number of the given channels (%zu, %zu) " "in the respective axis", s1, s0, smp->nch1, smp->nch2); /* p->imgss (image-sky-subtracted) is the sky subtracted input image. For both the removal of false detections and also the segmentation, it is important to use the sky subtracted image, not the actual input image for some operations. In both cases the input image is used for Signal to noise ratio measurements (where subtracting the sky will add noise). False detection removal: The sky subtracted image will be used for thresholding over the detected and undetected regions. Segmentation: The sky subtracted image will also be used for generating the catalog. Since both operations involve the sky subtracted input image (with different sky values) one array playing the role can really help in following the code. It will also help in the memory usage of the program. This array is allocated in the beginning and freed in the end and used throughout. A huge chunk of memory doesn't have to be allocated and de-allocated on every step. */ errno=0; p->imgss=malloc(s0*s1*sizeof *p->imgss); if(p->imgss==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->imgss in preparearrays " "(ui.c)", s0*s1*sizeof *p->imgss); /* Read the kernel: */ if(p->up.kernelnameset) gal_fits_prep_float_kernel(p->up.kernelname, p->up.khdu, &smp->kernel, &smp->ks0, &smp->ks1); else { errno=0; smp->ks0=defaultkernel_s0; smp->ks1=defaultkernel_s1; smp->kernel=malloc(smp->ks0*smp->ks1*sizeof *smp->kernel); if(smp->kernel==NULL) error(EXIT_FAILURE, errno, "%zu bytes for default kernel", smp->ks0*smp->ks1); ff=defaultkernel; fp=(f=smp->kernel)+smp->ks0*smp->ks1; do *f=*ff++; while(++fbyt=malloc(s0*s1*sizeof *p->byt); if(p->byt==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->byt (ui.c)", s0*s1*sizeof *p->byt); errno=0; p->olab=malloc(s0*s1*sizeof *p->olab); if(p->olab==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->olab (ui.c)", s0*s1*sizeof *p->olab); errno=0; p->clab=malloc(s0*s1*sizeof *p->clab); if(p->clab==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->clab (ui.c)", s0*s1*sizeof *p->clab); /* This ngb array is used to keep the relative indexs of the neighbors of a pixel. It is used in the over-segmentation step (clumps.c). The labelings are such that the first four elements are the four-connected ones and the second four are 8-connected. There is no problem with the negative values that are stored as size_t (which is an unsigned type): they will be added with positive values during the processing to give correct values. */ relngb[4]= s1-1; relngb[0]= s1; relngb[5]= s1+1; relngb[1]= -1; relngb[2]= 1; relngb[6]= -1*s1-1; relngb[3]= -1*s1; relngb[7]= -1*s1+1; /* Set the parameters for both mesh grids. */ lmp->s0=smp->s0; lmp->s1=smp->s1; lmp->ks0=smp->ks0; lmp->ks1=smp->ks1; lmp->nch1=smp->nch1; lmp->nch2=smp->nch2; lmp->kernel=smp->kernel; lmp->img=p->img=smp->img; lmp->params=smp->params=p; lmp->minmodeq=smp->minmodeq; lmp->mirrordist=smp->mirrordist; lmp->fullsmooth=smp->fullsmooth; lmp->numnearest=smp->numnearest; lmp->smoothwidth=smp->smoothwidth; lmp->lastmeshfrac=smp->lastmeshfrac; lmp->meshbasedcheck=smp->meshbasedcheck; lmp->interponlyblank=smp->interponlyblank; lmp->fullinterpolation=smp->fullinterpolation; lmp->numthreads=smp->numthreads=p->cp.numthreads; /* Prepare the mesh structures. */ gal_mesh_make_mesh(smp); gal_mesh_make_mesh(lmp); if(p->meshname) { gal_fits_array_to_file(p->meshname, "Input", FLOAT_IMG, smp->img, s0, s1, p->anyblank, p->wcs, NULL, SPACK_STRING); gal_mesh_check_mesh_id(smp, &meshindexs); gal_fits_array_to_file(p->meshname, "SmallMeshIndexs", LONG_IMG, meshindexs, s0, s1, 0, p->wcs, NULL, SPACK_STRING); free(meshindexs); gal_mesh_check_mesh_id(lmp, &meshindexs); gal_fits_array_to_file(p->meshname, "LargeMeshIndexs", LONG_IMG, meshindexs, s0, s1, 0, p->wcs, NULL, SPACK_STRING); free(meshindexs); } } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void setparams(int argc, char *argv[], struct noisechiselparams *p) { struct gal_commonparams *cp=&p->cp; /* Set the non-zero initial values, the structure was initialized to have a zero value for all elements. */ cp->spack = SPACK; cp->verb = 1; cp->numthreads = num_processors(NPROC_CURRENT); cp->removedirinfo = 1; /* NoiseChisel parameter initializations. */ p->detsnhistnbins=p->clumpsnhistnbins=0; /* Read the arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Add the user default values and save them if asked. */ GAL_CONFIGFILES_CHECK_SET_CONFIG; /* Check if all the required parameters are set. */ checkifset(p); /* Print the values for each parameter. */ if(cp->printparams) GAL_CONFIGFILES_REPORT_PARAMETERS_SET; /* Do a sanity check. */ sanitycheck(p); /* Make the array of input images. */ preparearrays(p); /* Everything is ready, notify the user of the program starting. */ if(cp->verb) { printf(SPACK_NAME" started on %s", ctime(&p->rawtime)); printf(" - Using %zu CPU thread%s\n", p->cp.numthreads, p->cp.numthreads==1 ? "." : "s."); printf(" - Input: %s (hdu: %s)\n", p->up.inputname, p->cp.hdu); if(p->up.maskname) printf(" - Mask: %s (hdu: %s)\n", p->up.maskname, p->up.mhdu); if(p->up.kernelnameset) printf(" - Kernel: %s (hdu: %s)\n", p->up.kernelname, p->up.khdu); else printf(" - Kernel: FWHM=2 pixel Gaussian.\n"); } } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void freeandreport(struct noisechiselparams *p, struct timeval *t1) { /* Free the allocated arrays: */ free(p->img); free(p->byt); free(p->olab); free(p->clab); free(p->imgss); free(p->cp.hdu); free(p->up.mhdu); free(p->up.khdu); free(p->cp.output); free(p->smp.kernel); free(p->up.kernelname); /* Free the mask image name. Note that p->up.inputname was not allocated, but given to the program by the operating system. */ if(p->up.maskname && p->up.maskname!=p->up.inputname) free(p->up.maskname); /* Free all the allocated names. Note that detsnhist */ free(p->skyname); free(p->meshname); free(p->threshname); free(p->maskdetname); free(p->detectionname); free(p->segmentationname); free(p->detectionskyname); /* Free the WCS structure: */ if(p->wcs) wcsvfree(&p->nwcs, &p->wcs); /* Print the final message. */ if(p->cp.verb) gal_timing_report(t1, SPACK_NAME" finished in", 0); } gnuastro-0.2.33-8a3b/bin/noisechisel/cite.h0000644000175000017500000000317212750745735015311 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CITE_H #define CITE_H #define NOISECHISELBIBTEX "" #define PRINTCITEABORT { \ printf("\nWe hope %s has been useful for your research.\n" \ "Citations are vital for the continued work on %s.\n" \ "Thank you for citing it in your research paper.\n" \ "\nPlease cite as \"%s\":\n\n%s\n\n%s", \ SPACK_NAME, SPACK_NAME, SPACK_STRING, \ GAL_STRINGS_MAIN_BIBTEX, NOISECHISELBIBTEX); \ exit(EXIT_SUCCESS); \ } #endif gnuastro-0.2.33-8a3b/bin/noisechisel/main.h0000644000175000017500000001743212774160133015302 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include #include #include /* Progarm name macros: */ #define SPACK "astnoisechisel" /* Subpackage executable name. */ #define SPACK_NAME "NoiseChisel" /* Subpackage full name. */ #define SPACK_STRING SPACK_NAME" ("PACKAGE_NAME") "PACKAGE_VERSION struct uiparams { char *inputname; /* Name of input file. */ char *maskname; /* Name of mask image file. */ char *mhdu; /* Name of mask image header name. */ char *kernelname; /* Name of kernel image file. */ char *khdu; /* Name of kernel header name. */ int fullconvolutionset; int fullinterpolationset; int fullsmoothset; int masknameset; int mhduset; int kernelnameset; int khduset; int skysubtractedset; int grownclumpsset; int smeshsizeset; int lmeshsizeset; int nch1set; int nch2set; int lastmeshfracset; int numnearestset; int smoothwidthset; int mirrordistset; int minmodeqset; int qthreshset; int erodeset; int erodengbset; int noerodequantset; int openingset; int openingngbset; int minbfracset; int sigclipmultipset; int sigcliptoleranceset; int dthreshset; int detsnminareaset; int minnumfalseset; int detquantset; int detsnhistnbinsset; int dilateset; int segsnminareaset; int keepmaxnearriverset; int segquantset; int clumpsnhistnbinsset; int gthreshset; int minriverlengthset; int objbordersnset; }; struct noisechiselparams { /* Other structures: */ struct uiparams up; /* User interface parameters. */ struct gal_commonparams cp; /* Common parameters. */ struct gal_mesh_params smp; /* Smaller mesh grid of input image. */ struct gal_mesh_params lmp; /* Larger mesh grid of input image. */ /* Input: */ int nwcs; /* Number of WCS structures. */ struct wcsprm *wcs; /* Pointer to WCS structures. */ int bitpix; /* Input image bitpix value. */ int anyblank; /* ==1 There are blank pixels in input image. */ int skysubtracted; /* ==1: the input image is already sky subted. */ /* output: */ char *meshname; /* Name of --checkmesh output. */ char *threshname; /* !=NULL: Name of threshold steps. */ char *detectionname; /* !=NULL: Name of detection steps. */ char *detectionskyname; /* !=NULL: Name of detection sky steps. */ char *detectionsnhist; /* !=NULL: Name of detection S/N histogram. */ char *skyname; /* !=NULL: Name of image showing sky and STD. */ char *segmentationname; /* !=NULL: Name of segmentation steps. */ char *clumpsnhist; /* !=NULL: Name of clump S/N histogram. */ int detectonly; /* ==1: Only do detection, no segmentation. */ char *maskdetname; /* !=NULL: Save masked detections and sky. */ int grownclumps; /* ==1: Save the grown clumps in output. */ /* Detection: */ float *conv; /* Convolved image. */ float qthresh; /* Quantile threshold on convolved img. */ float noerodequant; /* Quantile for no erosion. */ size_t erode; /* Number of times to erode thresholded image. */ int erodengb; /* Use 4 or 8 connectivity in erosion. */ size_t opening; /* Depth of opening to apply to eroded image. */ int openingngb; /* Use 4 or 8 connectivity in opening. */ float minbfrac; /* Minimum fraction of undetected pixels. */ float sigclipmultip; /* Multiple of standard deviation, sigma clip. */ float sigcliptolerance; /* Tolerance in sigma clip. */ float dthresh; /* Threshold to remove false detections. */ size_t detsnminarea; /* Minimum area to calculate S/N for detection.*/ size_t minnumfalse; /* Min No. false detections/segments for quant.*/ float detquant; /* False detection S/N quantile to find true. */ size_t detsnhistnbins; /* ==1: Save false detection S/Ns histogram. */ size_t dilate; /* Number of times to dilate true detections. */ /* Segmentation: */ size_t segsnminarea; /* Minimum area to find the S/N of a clump. */ float segquant; /* S/N quantile for true clump. */ size_t clumpsnhistnbins; /* ==1: Save false clumps S/Ns histogram. */ int keepmaxnearriver; /* ==1: Keep clumps with max touching river. */ float gthresh; /* Threshold to stop growing objects. */ size_t minriverlength; /* Minimum length of river between grown clmps.*/ float objbordersn; /* S/N of rivers to define objects. */ /* Operating mode: */ /* Internal: */ double detsn; /* Signal to noise threshold for detections. */ double clumpsn; /* Signal to noise threshold for clumps. */ float *img; /* Input image. */ float *imgss; /* Sky subtracted image. */ time_t rawtime; /* Starting time of the program. */ long *olab; /* Object labels. */ long *clab; /* Clump labels. */ unsigned char *byt; /* Array of single bytes for binary operations.*/ unsigned char *dbyt; /* False detection removal thresholded array. */ float minstd; /* For correction to counts per second data. */ float maxstd; /* To store in output header. */ float medstd; /* Median Standard deviation over image. */ float cpscorr; /* correction to counts per second data. */ unsigned char b0f1; /* ==1: we are now working on data, not noise. */ int stepnum; /* Number of step if user wants to see steps. */ size_t numobjects; /* Total number of objects (detections). */ size_t numclumps; /* Total number of clumps. */ size_t relngb[8]; /* Indexs of relative neighbors. */ size_t *numclumpsarr; /* The number of clumps in each mesh. */ float **sntablearr; /* Array of pointers to sntable of each mesh. */ }; #endif gnuastro-0.2.33-8a3b/bin/noisechisel/main.c0000644000175000017500000000325112774157757015311 00000000000000/********************************************************************* NoiseChisel - Detect and segment signal in noise. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include /* Includes time.h and sys/time.h */ #include "main.h" #include "ui.h" /* needs main.h. */ #include "noisechisel.h" /* needs main.h. */ int main (int argc, char *argv[]) { struct timeval t1; struct noisechiselparams p={{0}, {0}, {0}, {0}, 0}; /* Set the starting time. */ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ setparams(argc, argv, &p); /* Run MakeProfiles */ noisechisel(&p); /* Free all non-freed allocations. */ freeandreport(&p, &t1); /* Return successfully.*/ return EXIT_SUCCESS; } gnuastro-0.2.33-8a3b/bin/noisechisel/Makefile.in0000644000175000017500000017426413004464627016263 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY, to the extent permitted by law; without # even the implied warranty of MERCHANTABILITY or FITNESS FOR A # PARTICULAR PURPOSE. @SET_MAKE@ VPATH = @srcdir@ am__is_gnu_make = { \ if test -z '$(MAKELEVEL)'; then \ false; \ elif test -n '$(MAKE_HOST)'; then \ true; \ elif test -n '$(MAKE_VERSION)' && test -n '$(CURDIR)'; then \ true; \ else \ false; \ fi; \ } am__make_running_with_option = \ case $${target_option-} in \ ?) ;; \ *) echo "am__make_running_with_option: internal error: invalid" \ "target option '$${target_option-}' specified" >&2; \ exit 1;; \ esac; \ has_opt=no; \ sane_makeflags=$$MAKEFLAGS; \ if $(am__is_gnu_make); then \ sane_makeflags=$$MFLAGS; \ else \ case $$MAKEFLAGS in \ *\\[\ \ ]*) \ bs=\\; \ sane_makeflags=`printf '%s\n' "$$MAKEFLAGS" \ | sed "s/$$bs$$bs[$$bs $$bs ]*//g"`;; \ esac; \ 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GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ 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The name and value should be separated by # atleast one of the following charaacters: # space, `,`, `=` or `:` # # Run with `--help` option or read the manual for a full # explanation of what each option means. # # NOTE I: All counting is from zero, not one. # NOTE II: Lines starting with `#` are ignored. # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Input: hdu 0 khdu 0 skysubtracted 0 minbfrac 0.5 minnumfalse 100 # Output: grownclumps 0 # Mesh grid: smeshsize 32 lmeshsize 200 nch1 1 nch2 1 lastmeshfrac 0.51 numnearest 10 smoothwidth 3 fullconvolution 0 fullinterpolation 0 fullsmooth 0 # Detection: mirrordist 1.5 minmodeq 0.49 qthresh 0.3 erode 2 erodengb 4 noerodequant 0.9331 opening 1 openingngb 8 sigclipmultip 3 sigcliptolerance 0.2 dthresh -0.1 detsnminarea 15 detsnhistnbins 0 detquant 0.95 dilate 3 # Segmentation segsnminarea 25 keepmaxnearriver 0 segquant 0.95 clumpsnhistnbins 0 gthresh 0.5 minriverlength 15 objbordersn 1gnuastro-0.2.33-8a3b/bin/noisechisel/Makefile.am0000644000175000017500000000314512765246730016245 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. NOTE: $(top_srcdir)/bootstrapped/lib is only necessary ## for internally compiled utilities and libraries. It must not be included ## during the tests since the bootstrapped libraries are not installed. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Utility and its sources bin_PROGRAMS = astnoisechisel astnoisechisel_SOURCES = main.c main.h cite.h ui.c ui.h args.h \ noisechisel.c noisechisel.h thresh.c thresh.h binary.c binary.h \ label.c label.h detection.c detection.h sky.c sky.h segmentation.c \ segmentation.h clumps.c clumps.h astnoisechisel_LDADD = $(top_builddir)/bootstrapped/lib/libgnu.la \ -lgnuastro ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astnoisechisel.conf gnuastro-0.2.33-8a3b/bin/mkprof/0000755000175000017500000000000013004464725013250 500000000000000gnuastro-0.2.33-8a3b/bin/mkprof/cite.h0000644000175000017500000000316612750745735014305 00000000000000/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CITE_H #define CITE_H #define MKPROFBIBTEX "" #define PRINTCITEABORT { \ printf("\nWe hope %s has been useful for your research.\n" \ "Citations are vital for the continued work on %s.\n" \ "Thank you for citing it in your research paper.\n" \ "\nPlease cite as \"%s\":\n\n%s\n\n%s", \ SPACK_NAME, SPACK_NAME, SPACK_STRING, \ GAL_STRINGS_MAIN_BIBTEX, MKPROFBIBTEX); \ exit(EXIT_SUCCESS); \ } #endif gnuastro-0.2.33-8a3b/bin/mkprof/profiles.h0000644000175000017500000000270012753376260015171 00000000000000/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef PROFILES_H #define PROFILES_H double Gaussian(struct mkonthread *mkp); double totgaussian(double q); double Moffat(struct mkonthread *mkp); double moffat_alpha(double fwhm, double beta); double totmoffat(double alpha, double beta, double q); double Sersic(struct mkonthread *mkp); double sersic_b(double n); double totsersic(double n, double re, double b, double q); double Circumference(struct mkonthread *mkp); double Flat(struct mkonthread *mkp); #endif gnuastro-0.2.33-8a3b/bin/mkprof/profiles.c0000644000175000017500000000774112753376276015205 00000000000000/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include /* For total Sersic brightness. */ #include "main.h" #include "mkprof.h" /* Needs main.h, astrthreads.h */ #include "profiles.h" /**************************************************************** ***************** Profiles: ******************** ****************************************************************/ /* The Gaussian function at a point: junk is only used here to make it conform to the general format of functions in this file: like Sersic(). */ double Gaussian(struct mkonthread *mkp) { return exp( mkp->gaussian_c * mkp->r * mkp->r ); } /* The integral of the Gaussian from -inf to +inf equals the square root of PI. So from zero to +inf it equals half of that.*/ double totgaussian(double q) { return q*sqrt(M_PI)/2; } /* This function will find the moffat function alpha value based on the explantions here: http://labs.adsabs.harvard.edu/adsabs/abs/2001MNRAS.328..977T/ alpha=(FWHM/2)/(2^(1.0/beta)-1)^(0.5). Then the moffat function at r is: (1.0 + (r/alpha)^2.0)^(-1.0*beta)*/ double moffat_alpha(double fwhm, double beta) { return (fwhm/2)/pow((pow(2, 1/beta)-1), 0.5f); } /* Find the total value of the Moffat profile. I am using equation 10 from Pengetal 2010 (Galfit). In finding the profiles, I am assuming \Sigma_0=1. So that is what I put here too.*/ double totmoffat(double alpha, double beta, double q) { return M_PI*alpha*alpha*q/(beta-1); } /* Find the Moffat profile for a certain radius. rda=r/alpha and nb=-1*b. This is done before hand to speed up the process. */ double Moffat(struct mkonthread *mkp) { return pow(1+mkp->r*mkp->r/mkp->moffat_alphasq, mkp->moffat_nb); } /* This approximation of b(n) for n>0.35 is taken from McArthur, Courteau and Holtzman 2003: http://adsabs.harvard.edu/abs/2003ApJ...582..689 */ double sersic_b(double n) { if(n<=0.35f) error(EXIT_FAILURE, 0, "the Sersic index cannot be smaller " "than 0.35. It is %.3f", n); return 2*n-(1/3)+(4/(405*n))+(46/(25515*n*n))+ (131/(1148175*n*n*n)-(2194697/(30690717750*n*n*n*n))); } /* Find the Sersic profile for a certain radius. rdre=r/re, inv_n=1/n, nb= -1*b. */ double Sersic(struct mkonthread *mkp) { return exp( mkp->sersic_nb * ( pow(mkp->r/mkp->sersic_re, mkp->sersic_inv_n) -1 ) ); } /* Find the total brightness in a Sersic profile. From equation 4 in Peng 2010. This assumes the surface brightness at the effective radius is 1.*/ double totsersic(double n, double re, double b, double q) { return (2*M_PI*re*re*exp(b)*n*pow(b, -2*n)*q* gsl_sf_gamma(2*n)); } /* Make a circumference (inner to the radius). */ double Circumference(struct mkonthread *mkp) { return mkp->r > mkp->intruncr ? mkp->fixedvalue : 0.0f; } /* Always returns a fixed value: */ double Flat(struct mkonthread *mkp) { return mkp->fixedvalue; } gnuastro-0.2.33-8a3b/bin/mkprof/oneprofile.h0000644000175000017500000000221612616616510015503 00000000000000/******************************************************************** MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef ONEPROFILE_H #define ONEPROFILE_H int ispsf(double fcolvalue); void setprofparams(struct mkonthread *mkp); void makeoneprofile(struct mkonthread *mkp); #endif gnuastro-0.2.33-8a3b/bin/mkprof/oneprofile.c0000644000175000017500000003776113001632540015501 00000000000000/******************************************************************** MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include /* generate random seed */ #include /* used in setrandoms */ #include /* To make noise. */ #include /* gsl_integration_qng */ #include #include #include #include #include #include #include "main.h" #include "mkprof.h" /* Needs main.h and astrthreads.h */ #include "profiles.h" #include "oneprofile.h" /**************************************************************** ************** Elliptical radius ****************** ****************************************************************/ /* Convert cartesian coordinates to the rotated elliptical radius. */ void r_el(struct mkonthread *mkp) { double c=mkp->c, s=mkp->s, q=mkp->q, x=mkp->x, y=mkp->y; mkp->r = sqrt( (x*c+y*s)*(x*c+y*s) + ((y*c-x*s)*(y*c-x*s)/q/q) ); } /* Calculate the cercular distance of a pixel to the profile center. */ float r_circle(size_t p, struct mkonthread *mkp) { double x, y; x = p/mkp->width[0]; /* Note that width[0] is the First FITS */ y = p%mkp->width[0]; /* axis, not first C axis. */ return sqrt( (x-mkp->xc)*(x-mkp->xc) + (y-mkp->yc)*(y-mkp->yc) ); } /**************************************************************** ************** Random points ****************** ****************************************************************/ /* Fill pixel with random values */ float randompoints(struct mkonthread *mkp) { double xrange, yrange, sum=0.0f; size_t i, numrandom=mkp->p->numrandom; /* Set the range of the x and y: */ xrange=mkp->xh-mkp->xl; yrange=mkp->yh-mkp->yl; /* Find the sum of the profile on the random positions */ for(i=0;ix = mkp->xl + gsl_rng_uniform(mkp->rng)*xrange; mkp->y = mkp->yl + gsl_rng_uniform(mkp->rng)*yrange; r_el(mkp); sum+=mkp->profile(mkp); } return sum/numrandom; } /**************************************************************** ***************** 2D integration ******************** ****************************************************************/ /* This function is used in the integration of a profile. It assumes a fixed y and integrates over a range of x values. */ double twod_over_x(double x, void *params) { struct mkonthread *mkp=(struct mkonthread *) params; mkp->x=x; r_el(mkp); return mkp->profile(mkp); } /* Find the 2d integration over the region. */ double twod_over_xy(double y, void *params) { gsl_function F; static double abserr; static size_t neval=0; double epsabs=0, epsrel=EPSREL_FOR_INTEG, result; struct mkonthread *mkp=(struct mkonthread *) params; F.function = &twod_over_x; F.params = params; mkp->y=y; gsl_integration_qng(&F, mkp->xl, mkp->xh, epsabs, epsrel, &result, &abserr, &neval); return result; } /* 2D integration of a profile.*/ double integ2d(struct mkonthread *mkp) { gsl_function F; static double abserr; static size_t neval=0; double epsabs=0, epsrel=EPSREL_FOR_INTEG, result; F.function = &twod_over_xy; F.params = mkp; gsl_integration_qng(&F, mkp->yl, mkp->yh, epsabs, epsrel, &result, &abserr, &neval); return result; } /**************************************************************/ /************ Pixel by pixel building *************/ /********* Positions are in C not FITS *********/ /**************************************************************/ void makepixbypix(struct mkonthread *mkp) { float circ_r; struct gal_linkedlist_sll *Q=NULL; unsigned char *byt; float *img=mkp->ibq->img; int use_rand_points=1, ispeak=1; struct builtqueue *ibq=mkp->ibq; size_t is1=mkp->width[0], is0=mkp->width[1]; size_t p, ngb[4], *ind=&p, numngb, *n, *nf, x, y; double tolerance=mkp->p->tolerance, pixfrac, junk; double (*profile)(struct mkonthread *)=mkp->profile; double xc=mkp->xc, yc=mkp->yc, os=mkp->p->oversample; double truncr=mkp->truncr, approx, hp=mkp->p->halfpixel; /* lQ: Largest. sQ: Smallest in queue */ struct gal_linkedlist_tosll *lQ=NULL, *sQ; /* Find the nearest pixel to the profile center and add it to the queue. */ pixfrac = modf(mkp->xc, &junk); x=(long)mkp->xc + ( pixfrac<0.5f ? 0 : 1 ); pixfrac = modf(mkp->yc, &junk); y=(long)mkp->yc + ( pixfrac<0.5f ? 0 : 1 ); p=x*mkp->width[0]+y; /* If this is a point source, just fill that one pixel and go. */ if(mkp->type==POINTCODE) { img[p]=1; return; } /* Allocate the byt array to not repeat completed pixels. */ errno=0; byt=calloc(is0*is1, sizeof *byt); if(byt==NULL) error(EXIT_FAILURE, 0, "%zu bytes for map of object in row %zu of " "data in %s", is0*is1*sizeof *byt, ibq->id, mkp->p->up.catname); /* Start the queue: */ byt[p]=1; gal_linkedlist_add_to_tosll_end( &lQ, &sQ, p, r_circle(p, mkp) ); /* If random points are necessary, then do it: */ if(mkp->type==SERSICCODE || mkp->type==MOFFATCODE || mkp->type==GAUSSIANCODE) { while(sQ) { /* In case you want to see the status of the twosided ordered queue, increasing and decreasing side by side, uncomment this line. Note that there will be a lot of lines printed! */ /*print_tossll(lQ, sQ);*/ /* Pop the pixel from the queue and check if it is within the truncation radius. Note that `xc` and `p` both belong to the over sampled image. But all the profile parameters are in the non-oversampled image. So we divide the distance by os (p->oversample in double type) */ gal_linkedlist_pop_from_tosll_start(&lQ, &sQ, ind, &circ_r); /* ind=&p */ mkp->x=(p/is1-xc)/os; mkp->y=(p%is1-yc)/os; r_el(mkp); if(mkp->r>truncr) continue; /* Find the value for this pixel: */ mkp->xl=mkp->x-hp; mkp->xh=mkp->x+hp; mkp->yl=mkp->y-hp; mkp->yh=mkp->y+hp; /* printf("Center (%zu, %zu). r: %.4f. x: [%.4f--%.4f], " "y: [%.4f, %.4f]\n", p%is1+1, p/is1+1, mkp->r, mkp->xl, mkp->xh, mkp->yl, mkp->yh); */ /* Find the random points and profile center. */ img[p]=randompoints(mkp); approx=profile(mkp); if (fabs(img[p]-approx)/img[p] < tolerance) use_rand_points=0; /* Save the peak flux if this is the first pixel: */ if(ispeak) { mkp->peakflux=img[p]; ispeak=0; } /* For the log file: */ ++ibq->numaccu; ibq->accufrac+=img[p]; /* printf("\tac: %f, ap: %f, frac: %f\n", img[p], approx, fabs(img[p]-approx)/img[p]); gal_fits_array_to_file("tmp.fits", "", FLOAT_IMG, img, is0, is1, NULL, SPACK_STRING); */ /* Go over the neighbours and add them to queue of elements to check. */ GAL_NEIGHBORS_FILL_4_ALLIMG; nf=(n=ngb)+numngb; do if(byt[*n]==0) { byt[*n]=1; gal_linkedlist_add_to_tosll_end( &lQ, &sQ, *n, r_circle(*n, mkp) ); } while(++nx=(p/is1-xc)/os; mkp->y=(p%is1-yc)/os; r_el(mkp); if(mkp->r>truncr) { /* For the circumference, if the profile is too elongated and circumwidth is too small, then some parts of the circumference will not be shown without this condition. */ if(mkp->type==CIRCUMFERENCECODE) img[p]=profile(mkp); continue; } /* Find the value for this pixel: */ img[p]=profile(mkp); /* Save the peak flux if this is the first pixel: */ if(ispeak) { mkp->peakflux=img[p]; ispeak=0; } /* gal_fits_array_to_file("tmp.fits", "", FLOAT_IMG, img, is0, is1, NULL, SPACK_STRING); */ /* Go over the neighbours and add them to queue of elements to check. */ GAL_NEIGHBORS_FILL_4_ALLIMG; nf=(n=ngb)+numngb; do if(byt[*n]==0) { byt[*n]=1; gal_linkedlist_add_to_sll(&Q, *n); } while(++np; double *cat, sigma; int tp=p->tunitinp; size_t rcol=p->rcol, tcol=p->tcol; /* Fill in the profile independant parameters. */ cat=&p->cat[mkp->ibq->id*p->cs1]; cat[p->xcol] += p->shift[0]/p->oversample; cat[p->ycol] += p->shift[1]/p->oversample; mkp->c = cos((90-cat[p->pcol])*DEGREESTORADIANS); mkp->s = sin((90-cat[p->pcol])*DEGREESTORADIANS); mkp->q = cat[p->qcol]; mkp->brightness = pow( 10, (p->zeropoint - cat[p->mcol]) / 2.5f ); mkp->ibq->ispsf = ispsf(cat[p->fcol]); mkp->type = mkp->ibq->type=cat[p->fcol]; /* Fill the profile dependent parameters. */ switch (mkp->type) { case SERSICCODE: mkp->correction = 1; mkp->profile = &Sersic; mkp->sersic_re = cat[rcol]; mkp->sersic_inv_n = 1.0f/cat[p->ncol]; mkp->sersic_nb = -1.0f*sersic_b(cat[p->ncol]); mkp->truncr = tp ? cat[tcol] : cat[tcol]*cat[rcol]; break; case MOFFATCODE: mkp->correction = 1; mkp->profile = &Moffat; mkp->moffat_nb = -1.0f*cat[p->ncol]; mkp->moffat_alphasq = moffat_alpha(cat[rcol], cat[p->ncol]); mkp->moffat_alphasq *= mkp->moffat_alphasq; mkp->truncr = tp ? cat[tcol] : cat[tcol]*cat[rcol]/2; if(p->psfinimg==0 && p->individual==0) { mkp->brightness = 1.0f; /* When the PSF is a separate image, */ cat[p->xcol] = 0.0f; /* it should be centered and have a */ cat[p->ycol] = 0.0f; /* total brightness of 1.0f. */ } break; case GAUSSIANCODE: mkp->correction = 1; mkp->profile = &Gaussian; sigma = cat[rcol]/2.35482f; mkp->gaussian_c = -1.0f/(2.0f*sigma*sigma); mkp->truncr = tp ? cat[tcol] : cat[tcol]*cat[rcol]/2; if(p->psfinimg==0 && p->individual==0) { mkp->brightness = 1.0f; /* Same as the explanations for */ cat[p->xcol] = 0.0f; /* The Moffat profile. */ cat[p->ycol] = 0.0f; } break; case POINTCODE: mkp->correction = 1; mkp->fixedvalue = 1.0f; mkp->profile = &Flat; break; case FLATCODE: mkp->profile = &Flat; mkp->truncr = tp ? cat[tcol] : cat[tcol]*cat[rcol]; if(p->mforflatpix) { mkp->correction = 0; mkp->fixedvalue = cat[p->mcol]; } else { mkp->correction = 1; mkp->fixedvalue = 1.0f; } break; case CIRCUMFERENCECODE: mkp->profile = &Circumference; mkp->truncr = tp ? cat[tcol] : cat[tcol]*cat[rcol]; mkp->intruncr = mkp->truncr - p->circumwidth; if(p->mforflatpix) { mkp->correction = 0; mkp->fixedvalue = cat[p->mcol]; } else { mkp->correction = 1; mkp->fixedvalue = 1.0f; } if(mkp->intruncr<0.0f) mkp->intruncr = 0.0f; break; default: error(EXIT_FAILURE, 0, "a bug in setprofparams (oneprofile.c)! " "The profile code is not recognized. This should have been " "seen and reported prior to this step. Please contact us so " "we can correct this"); } } /**************************************************************/ /************ Outside functions *************/ /**************************************************************/ void makeoneprofile(struct mkonthread *mkp) { struct mkprofparams *p=mkp->p; float sum; size_t size; long os=p->oversample; double pixfrac, intpart; double *cat=&p->cat[ mkp->ibq->id*p->cs1 ]; /* Find the profile center (see comments above). mkp->width is in the non-oversampled scale.*/ pixfrac = modf(fabs(cat[p->xcol]), &intpart); mkp->yc = ( os * (mkp->width[0]/2 + pixfrac) + (pixfrac<0.50f ? os/2 : -1*os/2-1) ); mkp->yc = round(mkp->yc*100)/100; pixfrac = modf(fabs(cat[p->ycol]), &intpart); mkp->xc = ( os*(mkp->width[1]/2 + pixfrac) + (pixfrac<0.5f ? os/2 : -1*os/2-1) ); mkp->xc = round(mkp->xc*100)/100; /* From this point on, the widths are the actual pixel widths (with onversampling). */ mkp->width[0] *= os; mkp->width[1] *= os; mkp->ibq->imgwidth=mkp->width[0]; /* Allocate and clear the array for this one profile. */ errno=0; size=mkp->width[0]*mkp->width[1]; mkp->ibq->img=calloc(size, sizeof *mkp->ibq->img); if(mkp->ibq->img==NULL) error(EXIT_FAILURE, 0, "%zu bytes for object in row %zu of data in %s", size*sizeof *mkp->ibq->img, mkp->ibq->id, mkp->p->up.catname); /* Build the profile in the image. */ makepixbypix(mkp); /* Correct the sum of pixels in the profile so it has the fixed total magnitude or pixel value, mkp->correction was set in setprofparams. Note that the profiles were not normalized during the building.*/ if(mkp->correction) { /* First get the sum of all the pixels in the profile. */ sum=gal_statistics_float_sum(mkp->ibq->img, size); /* Correct the fraction of brightness that was calculated accurately (not using the pixel center). */ mkp->ibq->accufrac /= sum; /* Correct all the profile pixels. */ if(p->magatpeak) gal_array_fmultip_const(mkp->ibq->img, size, mkp->brightness/mkp->peakflux); else gal_array_fmultip_const(mkp->ibq->img, size, mkp->brightness/sum); } } gnuastro-0.2.33-8a3b/bin/mkprof/args.h0000644000175000017500000003415013003710030014256 00000000000000/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef ARGS_H #define ARGS_H #include #include /* Definition parameters for the argp: */ const char *argp_program_version=SPACK_STRING"\n"GAL_STRINGS_COPYRIGHT "\n\nWritten by Mohammad Akhlaghi"; const char *argp_program_bug_address=PACKAGE_BUGREPORT; static char args_doc[] = "[BackgroundImage] Catalog"; const char doc[] = /* Before the list of options: */ GAL_STRINGS_TOP_HELP_INFO SPACK_NAME" will create a FITS image containing any number of mock " "astronomical profiles based on an input catalog. All the profiles " "will be built from the center outwards. First by Monte Carlo " "integration, then using the central pixel position. The tolerance " "level specifies when to switch to a latter.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /* Available letters (-V which is used by GNU is also removed): a d f g j k l u v A B E G H I J L M O Q U W Z Maximum integer used so far: 517 */ static struct argp_option options[] = { { 0, 0, 0, 0, "Operating modes:", -1 }, { 0, 0, 0, 0, "Input:", 1 }, { 0, 0, 0, 0, "Output:", 2 }, { "naxis1", 'x', "INT", 0, "Number of pixels along first FITS axis.", 2 }, { "naxis2", 'y', "INT", 0, "Number of pixels along second FITS axis.", 2 }, { "inputascanvas", 'C', 0, 0, "Use input image for output size and WCS.", 2 }, { "oversample", 's', "INT", 0, "Scale of oversampling.", 2 }, { "psfinimg", 509, 0, 0, "PSF profiles made with all in output image.", 2 }, { "individual", 'i', 0, 0, "Build all profiles separately.", 2 }, { "nomerged", 'm', 0, 0, "Do not create a merged image of all profiles.", 2 }, { "type", 'T', "STR", 0, "byte, short, long, longlong, float, double.", 2 }, { 0, 0, 0, 0, "Profiles:", 3 }, { "numrandom", 'r', "INT", 0, "No. of random points in Monte Carlo integration.", 3 }, { "tolerance", 't', "FLT", 0, "Tolerance to switch to less accurate method.", 3 }, { "tunitinp", 'p', 0, 0, "Truncation is in units of pixels, not radius.", 3 }, { "xshift", 'X', "FLT", 0, "Shift profile centers and enlarge image, X axis.", 3 }, { "yshift", 'Y', "FLT", 0, "Shift profile centers and enlarge image, Y axis.", 3 }, { "prepforconv", 'c', 0, 0, "Shift and expand based on first catalog PSF.", 3 }, { "zeropoint", 'z', "FLT", 0, "Magnitude zero point.", 3 }, { "circumwidth", 'w', "FLT", 0, "Width of circumference (inward) profiles", 3 }, { "replace", 'R', 0, 0, "Replace overlapping profile pixels, don't add.", 3 }, { "magatpeak", 515, 0, 0, "Magnitude is for peak pixel, not full profile.", 3 }, { "envseed", 'e', 0, 0, "Use GSL_RNG_SEED environment variable for seed.", 3 }, { 0, 0, 0, 0, "Catalog (column number, starting from zero):", 4 }, { "xcol", 500, "INT", 0, "Center along first FITS axis (horizontal).", 4 }, { "ycol", 501, "INT", 0, "Center along second FITS axis (vertical).", 4 }, { "racol", 516, "INT", 0, "Center right ascension.", 4 }, { "deccol", 517, "INT", 0, "Center declination.", 4 }, { "fcol", 502, "INT", 0, "Sersic (0), Moffat (1), Gaussian (2), Point (3),\n" "Flat (4), Circumference (5).", 4 }, { "rcol", 503, "INT", 0, "Effective radius or FWHM in pixels.", 4 }, { "ncol", 504, "INT", 0, "Sersic index or Moffat beta.", 4 }, { "pcol", 505, "INT", 0, "Position angle.", 4 }, { "qcol", 506, "INT", 0, "Axis ratio.", 4 }, { "mcol", 507, "INT", 0, "Magnitude.", 4 }, { "tcol", 508, "INT", 0, "Truncation in units of --rcol, unless --tunitinp.", 4 }, { "mforflatpix", 'F', 0, 0, "mcol is flat pixel value (when f is 4 or 5)", 4 }, { 0, 0, 0, 0, "WCS parameters:", 5 }, { "crpix1", 510, "FLT", 0, "Pixel coordinate of reference point (axis 1).", 5 }, { "crpix2", 511, "FLT", 0, "Pixel coordinate of reference point (axis 2).", 5 }, { "crval1", 512, "FLT", 0, "Right ascension at reference point (degrees).", 5 }, { "crval2", 513, "FLT", 0, "Declination at reference point (degrees).", 5 }, { "resolution", 514, "FLT", 0, "Resolution of image (arcseconds/pixel).", 5 }, {0} }; /* Parse a single option: */ static error_t parse_opt(int key, char *arg, struct argp_state *state) { size_t tmp; /* Save the arguments structure: */ struct mkprofparams *p = state->input; /* Set the pointer to the common parameters for all programs here: */ state->child_inputs[0]=&p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); switch(key) { /* Operating modes: */ case 509: p->psfinimg=1; break; case 'i': p->individual=1; break; /* Output: */ case 'x': gal_checkset_sizet_l_zero(arg, &tmp, "naxis1", key, p->cp.spack, NULL, 0); p->naxes[0]=tmp; p->up.naxis1set=1; break; case 'y': gal_checkset_sizet_l_zero(arg, &tmp, "naxis2", key, p->cp.spack, NULL, 0); p->naxes[1]=tmp; p->up.naxis2set=1; break; case 'C': p->up.inputascanvas=1; p->up.inputascanvasset=1; break; case 's': gal_checkset_sizet_l_zero(arg, &p->oversample, "oversample", key, p->cp.spack, NULL, 0); p->up.oversampleset=1; break; case 'm': p->nomerged=1; break; case 'w': gal_checkset_double_l_value(arg, &p->circumwidth, "circumwidth", key, p->cp.spack, MINCIRCUMWIDTH, NULL, 0); p->up.circumwidthset=1; break; case 'R': p->replace=1; p->up.replaceset=1; break; case 'T': gal_checkset_known_types(arg, &p->up.type, NULL, 0); p->up.typeset=1; break; /* Profiles: */ case 'r': gal_checkset_sizet_l_zero(arg, &p->numrandom, "numrandom", key, p->cp.spack, NULL, 0); p->up.numrandomset=1; break; case 't': gal_checkset_float_l_0(arg, &p->tolerance, "tolerance", key, p->cp.spack, NULL, 0); p->up.toleranceset=1; break; case 'z': gal_checkset_any_float(arg, &p->zeropoint, "zeropoint", key, p->cp.spack, NULL, 0); p->up.zeropointset=1; break; case 'p': p->tunitinp=1; p->up.tunitinpset=1; break; case 'c': p->up.prepforconv=1; p->up.prepforconvset=1; break; case 'X': gal_checkset_sizet_el_zero(arg, &tmp, "xshift", key, p->cp.spack, NULL, 0); p->shift[0]=tmp; p->up.xshiftset=1; break; case 'Y': gal_checkset_sizet_el_zero(arg, &tmp, "yshift", key, p->cp.spack, NULL, 0); p->shift[1]=tmp; p->up.yshiftset=1; break; case 515: p->magatpeak=1; break; case 'e': p->envseed=1; p->up.envseedset=1; break; /* Catalog */ case 500: gal_checkset_sizet_el_zero(arg, &p->xcol, "xcol", ' ', p->cp.spack, NULL, 0); p->up.xcolset=1; break; case 501: gal_checkset_sizet_el_zero(arg, &p->ycol, "ycol", ' ', p->cp.spack, NULL, 0); p->up.ycolset=1; break; case 516: gal_checkset_sizet_el_zero(arg, &p->racol, "racol", ' ', p->cp.spack, NULL, 0); p->up.racolset=1; break; case 517: gal_checkset_sizet_el_zero(arg, &p->deccol, "deccol", ' ', p->cp.spack, NULL, 0); p->up.deccolset=1; break; case 502: gal_checkset_sizet_el_zero(arg, &p->fcol, "fcol", ' ', p->cp.spack, NULL, 0); p->up.fcolset=1; break; case 503: gal_checkset_sizet_el_zero(arg, &p->rcol, "rcol", ' ', p->cp.spack, NULL, 0); p->up.rcolset=1; break; case 504: gal_checkset_sizet_el_zero(arg, &p->ncol, "ncol", ' ', p->cp.spack, NULL, 0); p->up.ncolset=1; break; case 505: gal_checkset_sizet_el_zero(arg, &p->pcol, "pcol", ' ', p->cp.spack, NULL, 0); p->up.pcolset=1; break; case 506: gal_checkset_sizet_el_zero(arg, &p->qcol, "qcol", ' ', p->cp.spack, NULL, 0); p->up.qcolset=1; break; case 507: gal_checkset_sizet_el_zero(arg, &p->mcol, "mcol", ' ', p->cp.spack, NULL, 0); p->up.mcolset=1; break; case 508: gal_checkset_sizet_el_zero(arg, &p->tcol, "tcol", ' ', p->cp.spack, NULL, 0); p->up.tcolset=1; break; case 'F': p->mforflatpix=1; p->up.mforflatpixset=1; break; /* WCS parameters: */ case 510: gal_checkset_any_double(arg, &p->crpix[0], "crpix1", key, p->cp.spack, NULL, 0); p->up.crpix1set=1; break; case 511: gal_checkset_any_double(arg, &p->crpix[1], "crpix2", key, p->cp.spack, NULL, 0); p->up.crpix2set=1; break; case 512: gal_checkset_any_double(arg, &p->crval[0], "crval1", key, p->cp.spack, NULL, 0); p->up.crval1set=1; break; case 513: gal_checkset_any_double(arg, &p->crval[1], "crval2", key, p->cp.spack, NULL, 0); p->up.crval2set=1; break; case 514: gal_checkset_float_l_0(arg, &p->resolution, "resolution", key, p->cp.spack, NULL, 0); p->up.resolutionset=1; break; /* Read the non-option arguments: */ case ARGP_KEY_ARG: /* See what type of input value it is and put it in. */ if( gal_fits_name_is_fits(arg) ) { if(p->up.backname) argp_error(state, "only one input FITS image (the background) " "should be input. You have given more"); else p->up.backname=arg; } else { if(p->up.catname) argp_error(state, "only one catalog file can be given"); else p->up.catname=arg; } break; /* The command line options and arguments are finished. */ case ARGP_KEY_END: if(p->cp.setdirconf==0 && p->cp.setusrconf==0 && p->cp.printparams==0) { if(state->arg_num==0) argp_error(state, "no argument given"); if(p->up.catname==NULL) argp_error(state, "no catalog provided"); } break; default: return ARGP_ERR_UNKNOWN; } return 0; } /* Specify the children parsers: */ struct argp_child children[]= { {&commonargp, 0, NULL, 0}, {0, 0, 0, 0} }; /* Basic structure defining the whole argument reading process. */ static struct argp thisargp = {options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif gnuastro-0.2.33-8a3b/bin/mkprof/mkprof.h0000644000175000017500000000727312764767045014665 00000000000000/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MOCKGALS_H #define MOCKGALS_H #include #include "main.h" struct mkonthread { /* General parameters: */ double r; /* Elliptical radius at this point. */ double x; /* x value of this point. */ double xl; /* lower x boundary */ double xh; /* higher x boundary. */ double y; /* y value when integrating over x. */ double yl; /* lower y boundary. */ double yh; /* higher y boundary. */ double c; /* Cosine of the position angle. */ double s; /* Sine of the position angle. */ double q; /* axis ratio of the position angle. */ double xc; /* Center in C of created(oversampled). */ double yc; /* Center in C of created(oversampled). */ double (*profile)(struct mkonthread *); /* Function to use. */ double truncr; /* Truncation radius in pixels. */ double intruncr; /* Inner truncation radius in pixels. */ long width[2]; /* The width of the enclosing box. */ float peakflux; /* Flux at profile peak. */ float brightness; /* The brightness of the profile. */ int type; /* The type of the profile. */ long *onaxes; /* Sides of the unover-sampled image. */ long fpixel_i[2]; /* fpixel_i before running overlap. */ int correction; /* ==1: correct the pixels afterwards. */ /* Random number generator: */ gsl_rng *rng; /* Copy of main random number generator. */ /* Profile specific parameters: */ double sersic_re; /* r/re in Sersic profile. */ double sersic_inv_n; /* Sersic index of Sersic profile. */ double sersic_nb; /* Negative of b(n) constant. */ double moffat_alphasq; /* r divided by alpha in Moffat. */ double moffat_nb; /* Negative beta in the Moffat. */ double gaussian_c; /* Constant value in Gaussian. */ double fixedvalue; /* Value of a point source. */ /* General parameters */ struct mkprofparams *p; /* Pointer to the main.h structure. */ size_t *indexs; /* Indexs to build on this thread. */ pthread_barrier_t *b; /* Pthread barrier pointer. */ struct builtqueue *ibq; /* Internally built queue. */ }; void mkprof(struct mkprofparams *p); #endif gnuastro-0.2.33-8a3b/bin/mkprof/mkprof.c0000644000175000017500000005070013001632540014621 00000000000000/******************************************************************** MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include "main.h" #include "mkprof.h" /* Needs main.h astrthreads.h */ #include "oneprofile.h" /**************************************************************/ /************ builtqueue linked list *************/ /**************************************************************/ /* Add an empty element to the existing builtqueue. */ void builtqueue_addempty(struct builtqueue **bq) { struct builtqueue *tbq; /* Allocate the element. */ errno=0; tbq=malloc(sizeof *tbq); if(tbq==NULL) error(EXIT_FAILURE, 0, "%zu byte element in builtqueue_addempty", sizeof *tbq); /* Initialize some of the values. */ tbq->img=NULL; tbq->numaccu=0; tbq->accufrac=0.0f; tbq->indivcreated=0; /* Set its next element to the input bq and re-set the input bq. */ tbq->next=*bq; *bq=tbq; } /**************************************************************/ /************ Save individual *************/ /**************************************************************/ #define NUMBERNAMESTRLEN 100 void saveindividual(struct mkonthread *mkp) { struct mkprofparams *p=mkp->p; size_t len; double crpix[2]; long os=p->oversample; struct builtqueue *ibq=mkp->ibq; char *outname, *jobname, *outdir=p->outdir; /* Allocate the space for the name of this file. */ errno=0; len=strlen(outdir)+NUMBERNAMESTRLEN+strlen(p->mergedimgname); outname=malloc(len*sizeof *outname); if(outname==NULL) error(EXIT_FAILURE, errno, "%zu bytes for name of object in " "row %zu of %s", len*sizeof *outname, ibq->id, p->up.catname); /* Save the correct CRPIX values: */ crpix[0] = p->crpix[0] - os*(mkp->fpixel_i[0]-1); crpix[1] = p->crpix[1] - os*(mkp->fpixel_i[1]-1); /* Write the name and remove a similarly named file. */ sprintf(outname, "%s%zu_%s", outdir, ibq->id, p->basename); gal_checkset_check_remove_file(outname, p->cp.dontdelete); /* Write the array to file (A separately built PSF doesn't need WCS coordinates): */ if(ibq->ispsf && p->psfinimg==0) gal_fits_array_to_file(outname, "MockImg", FLOAT_IMG, ibq->img, mkp->width[1], mkp->width[0], 0, NULL, NULL, SPACK_STRING); else gal_fits_atof_correct_wcs(outname, "MockImg", FLOAT_IMG, ibq->img, mkp->width[1], mkp->width[0], p->wcsheader, p->wcsnkeyrec, crpix, SPACK_STRING); ibq->indivcreated=1; /* Report if in verbose mode. */ if(p->cp.verb) { errno=0; jobname=malloc((len+100)*sizeof *jobname); if(jobname==NULL) error(EXIT_FAILURE, errno, "jobname in mkprof.c"); sprintf(jobname, "%s created.", outname); gal_timing_report(NULL, jobname, 2); free(jobname); } free(outname); } /**************************************************************/ /************ The builders *************/ /**************************************************************/ /* Build the profiles that are indexed in the indexs array of the mkonthread structure that was assigned to it. See the explanation above overlap (/lib/box.c) for a complete explanation of fpixel_i, lpixel_i, fpixel_o and lpixel_o. ========================================================= About the Central x and y of each profile: The user has asked for the profile to be built on the coordinates (real numbers) of `x` and `y` in an output image in the FITS format. We are building the full image for each galaxy separately in an array with an odd number of sides which maybe oversampled. In the FITS format, the pixel centers have an integer value. So for example in 1D, a pixel whose center value is 10.00 covers the area of: [9.5,10.5). We want the fractional part of `x` (don't forget, this example is 1D) to be in the central pixel of this separate array (with odd sides) that we will be building. The result of this convention is that in 1D, a continuous space pixel with a fractional value of 0.1 is going to be after the central pixel's center, while one with a fractional value of 0.9 will be before it. In this manner, later on, when we want to find the overlap between this array and the output array, if we have a fractional value >=0.5, we will just shift the integer part of the central pixel by one and completely ignore the fractional part. */ void * build(void *inparam) { struct mkonthread *mkp=(struct mkonthread *)inparam; struct mkprofparams *p=mkp->p; size_t i; double *cat; int lockresult; long lpixel_o[2]; pthread_mutex_t *qlock=&p->qlock; struct builtqueue *ibq, *fbq=NULL; pthread_cond_t *qready=&p->qready; /* Make each profile that was specified for this thread. */ for(i=0;mkp->indexs[i]!=GAL_THREADS_NON_THRD_INDEX;++i) { /* Create a new builtqueue element with all the information. fbq will be used when we want to add ibq to p->bq. It is defined so we don't have to waste time traversing the ibq. Its characteristic compared to the other elements of ibq is that fbq->next==NULL. So to add ibq to p->bq, we just have to set fbq->next=p->bq and then set p->bq to ibq.*/ builtqueue_addempty(&mkp->ibq); ibq=mkp->ibq; ibq->id=mkp->indexs[i]; if(fbq==NULL) fbq=ibq; cat=&p->cat[ibq->id*p->cs1]; /* Write the necessary parameters for this profile into mkp.*/ setprofparams(mkp); /* Find the bounding box size (NOT oversampled). */ if((int)cat[p->fcol]==POINTCODE) mkp->width[0]=mkp->width[1]=1; else gal_box_ellipse_in_box(mkp->truncr, mkp->q*mkp->truncr, cat[p->pcol]*DEGREESTORADIANS, mkp->width); /* Get the overlapping pixels using the starting points (NOT oversampled). */ gal_box_border_from_center(cat[p->xcol], cat[p->ycol], mkp->width, ibq->fpixel_i, ibq->lpixel_i); mkp->fpixel_i[0]=ibq->fpixel_i[0]; mkp->fpixel_i[1]=ibq->fpixel_i[1]; ibq->overlaps = gal_box_overlap(mkp->onaxes, ibq->fpixel_i, ibq->lpixel_i, ibq->fpixel_o, lpixel_o); /* Build the profile if necessary, After this, the width is oversampled. */ if(ibq->overlaps || p->individual || (ibq->ispsf && p->psfinimg==0)) { /* Put a copy of the main random number generator for this thread to use for this profile. */ gsl_rng_memcpy(mkp->rng, p->rng); /* Set the seed of the random number generator if the environment is not to be used. */ if(mkp->p->envseed==0) gsl_rng_set(mkp->rng, gal_timing_time_based_rng_seed()); /* Make the profile */ makeoneprofile(mkp); if( p->individual || (ibq->ispsf && p->psfinimg==0)) { saveindividual(mkp); if(ibq->ispsf && p->psfinimg==0) ibq->overlaps=0; } } /* Add ibq to bq if you can lock the mutex. */ if(p->cp.numthreads>1) { /* Try locking the mutex so no thread can change the value of p->bq. If you can lock it, then put the internal builtqueue on top of the general builtqueue. If you can't, continue adding to the internal builtqueue (make the next profiles) until you find a chance to lock the mutex. */ lockresult=pthread_mutex_trylock(qlock); if(lockresult==0) /* Mutex was successfully locked. */ { /* Add this internal queue to system queue. */ fbq->next=p->bq; p->bq=ibq; /* If the list was empty when you locked the mutex, then either `write` is waiting behind a condition variable for you to fill it up or not (either it hasn't got to setting the condition variable yet (this function locked the mutex before `write`) or it just got the list to be made and is busy writing the arrays in the output). In either case, pthread_cond_signal will work. */ if(fbq->next==NULL) pthread_cond_signal(qready); pthread_mutex_unlock(qlock); /* Finally set both the internal queue and the first internal queue element to NULL.*/ fbq=NULL; mkp->ibq=NULL; } /* The mutex couldn't be locked and there are no more objects for this thread to build (giving a chance for this thread to add up its built profiles). So we have to lock the mutex to pass on this built structure to the builtqueue. */ else if (mkp->indexs[i+1]==GAL_THREADS_NON_THRD_INDEX) { pthread_mutex_lock(qlock); fbq->next=p->bq; p->bq=ibq; pthread_cond_signal(qready); pthread_mutex_unlock(qlock); } } } /* Free the allocated space for this thread and wait until all other threads finish. */ gsl_rng_free(mkp->rng); if(p->cp.numthreads==1) p->bq=mkp->ibq; else pthread_barrier_wait(mkp->b); return NULL; } /**************************************************************/ /************ The writer *************/ /**************************************************************/ void writelog(struct mkprofparams *p) { int space[]={6, 10, 15}, prec[]={3, 6}; int int_cols[]={0, 2, 4, -1}, accu_cols[]={-1}; char comments[1000], gitdescribe[100], *gd=gal_git_describe(); if(gd) sprintf(gitdescribe, " from %s,", gd); else gitdescribe[0]='\0'; sprintf(comments, "# Log file for "SPACK_STRING".\n" "# Created%s on %s" "# Column 0: Row number in catalog (starting from zero).\n" "# Column 1: Overlap magnitude with final image " "(zeropoint: %.3f).\n" "# Column 2: Number of Monte Carlo integration pixels.\n" "# Column 3: Fraction of brightness in Monte Carlo " "integrated pixels.\n" "# Column 4: An individual image was created.\n", ctime(&p->rawtime), gitdescribe, p->zeropoint); gal_txtarray_array_to_txt(p->log, p->cs0, LOGNUMCOLS, comments, int_cols, accu_cols, space, prec, 'f', LOGFILENAME); } void write(struct mkprofparams *p) { void *array; char *jobname; double sum, *log; struct timeval t1; long os=p->oversample; int replace=p->replace; size_t complete=0, cs0=p->cs0; struct builtqueue *ibq=NULL, *tbq; int verb=p->cp.verb, bitpix=p->bitpix; float *out, *to, *from, *colend, *rowend; size_t i, j, iw, jw, ii, jj, w=p->naxes[0], ow; /* Allocate the output array if necessary. */ if(p->out) out=p->out; else { errno=0; out=calloc(p->naxes[0]*p->naxes[1], sizeof *out); if(out==NULL) error(EXIT_FAILURE, 0, "%zu bytes for output image", p->naxes[0]*p->naxes[1]*sizeof *out); } /* Write each image into the output array. */ while(completecs0) { /* Set ibq. */ if(ibq==NULL) { if(p->cp.numthreads==1) ibq=p->bq; else { pthread_mutex_lock(&p->qlock); while(p->bq==NULL) pthread_cond_wait(&p->qready, &p->qlock); ibq=p->bq; p->bq=NULL; pthread_mutex_unlock(&p->qlock); } } sum=0.0f; /* Write the array pointed to by ibq into the output image. Note that the FITS and C arrays have opposite axis orders and FITS counting starts from 1, not zero. Also fpixel is the first (inclusive) pixel and so is lpixel (it is inclusive). */ if(ibq->overlaps && p->nomerged==0) { /* Set the starting and ending points in the complete image. */ i = os * (ibq->fpixel_i[1]-1); j = os * (ibq->fpixel_i[0]-1); /* Set the starting and ending points in the overlapping image. Note that oversampling has already been taken into account in ibq->width. */ ow = ibq->imgwidth; ii = os * (ibq->fpixel_o[1]-1); jj = os * (ibq->fpixel_o[0]-1); /* Find the width of the overlapping region: */ iw = os*(ibq->lpixel_i[1]-ibq->fpixel_i[1]+1); jw = os*(ibq->lpixel_i[0]-ibq->fpixel_i[0]+1); /* Write the overlap to the actual image. Instead of writing two for loops and summing all the row and column indexs for every pixel and each image, we use pointer arithmetic which is much more efficient. Just think of one pointer that is advancing over the final image (*to) and one that is advancing over the overlap image (*from). Since we know the images overlap, iw and jw are both smaller than the two image number of columns and number of rows, so w-jw and ow-jw will always be positive. */ to=out+i*w+j; from=ibq->img+ii*ow+jj; rowend=to+iw*w; do { /* Go over all the pixels in this row and write this profile into the final output array. Just note that when replacing, we don't want to replace those pixels that have a zero value, since no profile existed there. */ colend=to+jw; do { *to = ( replace ? ( *from==0.0f ? *to : *from ) : *to + *from ); sum += *from; ++from; } while(++tolog[ibq->id*LOGNUMCOLS]; log[0] = ibq->id; log[1] = sum>0.0f ? -2.5f*log10(sum)+p->zeropoint : NAN; log[2] = ibq->numaccu; log[3] = ibq->accufrac; log[4] = ibq->indivcreated; /* Report if in verbose mode. */ ++complete; if(verb && p->nomerged==0) { errno=0; jobname=malloc(100*sizeof *jobname); if(jobname==NULL) error(EXIT_FAILURE, errno, "jobname in mkprof.c"); sprintf(jobname, "row %zu complete, %zu left to go", ibq->id, cs0-complete); gal_timing_report(NULL, jobname, 2); free(jobname); } /* Free the array and the queue element and change it to the next one and increment complete. Note that there is no problem to free a NULL pointer (when the built array didn't overlap). */ free(ibq->img); tbq=ibq->next; free(ibq); ibq=tbq; } /* Write the final array to the output FITS image. */ if(p->nomerged==0) { /* Get the current time for verbose output. */ if(verb) gettimeofday(&t1, NULL); /* Make a temporary array of the desired type for writing the output. */ if(bitpix==FLOAT_IMG) array=out; else gal_fits_change_type(out, FLOAT_IMG, p->naxes[1]*p->naxes[0], p->anyblank, &array, bitpix); /* Write the array to the output FITS file. */ gal_fits_array_to_file(p->mergedimgname, "Mock image", bitpix, array, p->naxes[1], p->naxes[0], p->anyblank, p->wcs, NULL, SPACK_STRING); /* Free `array' if it was allocated separately.*/ if(bitpix!=FLOAT_IMG) free(array); /* In verbose mode, print the information. */ if(verb) { errno=0; jobname=malloc((strlen(p->mergedimgname)+100)*sizeof *jobname); if(jobname==NULL) error(EXIT_FAILURE, errno, "final report in mkprof.c"); sprintf(jobname, "%s created.", p->mergedimgname); gal_timing_report(&t1, jobname, 1); free(jobname); } } free(out); } /**************************************************************/ /************ Outside function *************/ /**************************************************************/ void mkprof(struct mkprofparams *p) { int err; pthread_t t; /* Thread id not used, all are saved here. */ pthread_attr_t attr; pthread_barrier_t b; struct mkonthread *mkp; size_t i, *indexs, thrdcols; size_t nt=p->cp.numthreads, nb; long onaxes[2], os=p->oversample; /* Allocate the arrays to keep the thread and parameters for each thread. Note that we only want nt-1 threads to do the building. */ errno=0; mkp=malloc(nt*sizeof *mkp); if(mkp==NULL) error(EXIT_FAILURE, errno, "%zu bytes in mkprof (mkprof.c) for mkp", (nt-1)*sizeof *mkp); /* Distribute the different profiles for different threads. Note that one thread is left out for writing, while nt-1 are left for building. */ gal_threads_dist_in_threads(p->cs0, nt, &indexs, &thrdcols); /* onaxes are sides of the image without over-sampling. */ onaxes[0] = (p->naxes[0]-2*p->shift[0])/os + 2*p->shift[0]/os; onaxes[1] = (p->naxes[1]-2*p->shift[1])/os + 2*p->shift[1]/os; /* Build the profiles: */ if(nt==1) { mkp[0].p=p; mkp[0].onaxes=onaxes; mkp[0].indexs=indexs; mkp[0].rng=gsl_rng_clone(p->rng); build(&mkp[0]); } else { /* Initialize the attributes. Note that this main thread will also have to be kept behind the barrier, so we need nt+1 barrier stops. */ if(p->cs0cs0+1; else nb=nt+1; gal_threads_attr_barrier_init(&attr, &b, nb); /* Initialize the condition variable and mutex. */ err=pthread_mutex_init(&p->qlock, NULL); if(err) error(EXIT_FAILURE, 0, "mutex not initialized"); err=pthread_cond_init(&p->qready, NULL); if(err) error(EXIT_FAILURE, 0, "condition variable not initialized"); /* Spin off the threads: */ for(i=0;irng); mkp[i].indexs=&indexs[i*thrdcols]; err=pthread_create(&t, &attr, build, &mkp[i]); if(err) error(EXIT_FAILURE, 0, "can't create thread %zu", i); } } /* Write the created arrays into the image. */ write(p); if(p->cp.nolog==0) writelog(p); /* If numthreads>1, then wait for all the jobs to finish and destroy the attribute and barrier. */ if(nt>1) { pthread_barrier_wait(&b); pthread_attr_destroy(&attr); pthread_barrier_destroy(&b); pthread_cond_destroy(&p->qready); pthread_mutex_destroy(&p->qlock); } /* Free the allocated spaces. */ free(mkp); free(indexs); } gnuastro-0.2.33-8a3b/bin/mkprof/ui.h0000644000175000017500000000230312754550525013761 00000000000000/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef UI_H #define UI_H void checksaveouttype(struct mkprofparams *p, char *arg); void setparams(int argc, char *argv[], struct mkprofparams *p); void freeandreport(struct mkprofparams *p, struct timeval *t1); #endif gnuastro-0.2.33-8a3b/bin/mkprof/ui.c0000644000175000017500000010362013001632540013740 00000000000000/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* From Gnulib. */ #include #include #include #include #include #include #include /* Includes time.h and sys/time.h */ #include #include #include #include "main.h" #include "mkprof.h" #include "ui.h" /* Needs main.h. */ #include "args.h" /* Needs main.h, includes argp.h. */ #include "oneprofile.h" /* Needs main.h and mkprof.h. */ /* Set the file names of the places where the default parameters are put. */ #define CONFIG_FILE SPACK CONF_POSTFIX #define SYSCONFIG_FILE SYSCONFIG_DIR "/" CONFIG_FILE #define USERCONFIG_FILEEND USERCONFIG_DIR CONFIG_FILE #define CURDIRCONFIG_FILE CURDIRCONFIG_DIR CONFIG_FILE /**************************************************************/ /************** Options and parameters ***************/ /**************************************************************/ void readconfig(char *filename, struct mkprofparams *p) { FILE *fp; char *line, *name, *value; struct uiparams *up=&p->up; size_t lineno=0, len=200, tmp; struct gal_commonparams *cp=&p->cp; char key='a'; /* Not used, just a place holder. */ /* When the file doesn't exist or can't be opened, it is ignored. It might be intentional, so there is no error. If a parameter is missing, it will be reported after all defaults are read. */ fp=fopen(filename, "r"); if (fp==NULL) return; /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); /* Read the tokens in the file: */ while(getline(&line, &len, fp) != -1) { /* Prepare the "name" and "value" strings, also set lineno. */ GAL_CONFIGFILES_START_READING_LINE; /* Inputs: */ if(strcmp(name, "hdu")==0) gal_checkset_allocate_copy_set(value, &cp->hdu, &cp->hduset); /* Outputs: */ else if(strcmp(name, "output")==0) gal_checkset_allocate_copy_set(value, &cp->output, &cp->outputset); else if(strcmp(name, "naxis1")==0) { if(up->naxis1set) continue; gal_checkset_sizet_l_zero(value, &tmp, name, key, SPACK, filename, lineno); p->naxes[0]=tmp; up->naxis1set=1; } else if(strcmp(name, "inputascanvas")==0) { if(up->inputascanvasset) continue; gal_checkset_int_zero_or_one(value, &up->inputascanvas, name, key, SPACK, filename, lineno); up->inputascanvasset=1; } else if(strcmp(name, "naxis2")==0) { if(up->naxis2set) continue; gal_checkset_sizet_l_zero(value, &tmp, name, key, SPACK, filename, lineno); p->naxes[1]=tmp; up->naxis2set=1; } else if(strcmp(name, "oversample")==0) { if(up->oversampleset) continue; gal_checkset_sizet_l_zero(value, &p->oversample, name, key, SPACK, filename, lineno); up->oversampleset=1; } else if(strcmp(name, "replace")==0) { if(up->replaceset) continue; gal_checkset_int_zero_or_one(value, &p->replace, name, key, SPACK, filename, lineno); up->replaceset=1; } else if(strcmp(name, "type")==0) { if(p->up.typeset) continue; gal_checkset_known_types(value, &p->up.type, filename, lineno); p->up.typeset=1; } /* Profiles: */ else if(strcmp(name, "tunitinp")==0) { if(up->tunitinpset) continue; gal_checkset_int_zero_or_one(value, &p->tunitinp, name, key, SPACK, filename, lineno); up->tunitinpset=1; } else if(strcmp(name, "numrandom")==0) { if(up->numrandomset) continue; gal_checkset_sizet_l_zero(value, &p->numrandom, name, key, SPACK, filename, lineno); up->numrandomset=1; } else if(strcmp(name, "tolerance")==0) { if(up->toleranceset) continue; gal_checkset_float_l_0(value, &p->tolerance, name, key, SPACK, filename, lineno); up->toleranceset=1; } else if(strcmp(name, "zeropoint")==0) { if(up->zeropointset) continue; gal_checkset_any_float(value, &p->zeropoint, name, key, SPACK, filename, lineno); up->zeropointset=1; } else if(strcmp(name, "prepforconv")==0) { if(up->prepforconvset) continue; gal_checkset_int_zero_or_one(value, &p->up.prepforconv, name, key, SPACK, filename, lineno); up->prepforconvset=1; } else if(strcmp(name, "xshift")==0) { if(up->xshiftset) continue; gal_checkset_sizet_el_zero(value, &tmp, name, key, SPACK, filename, lineno); p->shift[0]=tmp; up->xshiftset=1; } else if(strcmp(name, "yshift")==0) { if(up->yshiftset) continue; gal_checkset_sizet_el_zero(value, &tmp, name, key, SPACK, filename, lineno); p->shift[1]=tmp; up->yshiftset=1; } else if(strcmp(name, "circumwidth")==0) { if(up->circumwidthset) continue; gal_checkset_double_l_value(value, &p->circumwidth, name, key, SPACK, MINCIRCUMWIDTH, filename, lineno); up->circumwidthset=1; } else if(strcmp(name, "envseed")==0) { if(up->envseedset) continue; gal_checkset_int_zero_or_one(value, &p->envseed, name, key, SPACK, filename, lineno); up->envseedset=1; } /* Catalog: */ else if(strcmp(name, "xcol")==0) { if(up->xcolset) continue; gal_checkset_sizet_el_zero(value, &p->xcol, name, key, SPACK, filename, lineno); up->xcolset=1; } else if(strcmp(name, "ycol")==0) { if(up->ycolset) continue; gal_checkset_sizet_el_zero(value, &p->ycol, name, key, SPACK, filename, lineno); up->ycolset=1; } else if(strcmp(name, "racol")==0) { if(up->racolset) continue; gal_checkset_sizet_el_zero(value, &p->racol, name, key, SPACK, filename, lineno); up->racolset=1; } else if(strcmp(name, "deccol")==0) { if(up->deccolset) continue; gal_checkset_sizet_el_zero(value, &p->deccol, name, key, SPACK, filename, lineno); up->deccolset=1; } else if(strcmp(name, "fcol")==0) { if(up->fcolset) continue; gal_checkset_sizet_el_zero(value, &p->fcol, name, key, SPACK, filename, lineno); up->fcolset=1; } else if(strcmp(name, "rcol")==0) { if(up->rcolset) continue; gal_checkset_sizet_el_zero(value, &p->rcol, name, key, SPACK, filename, lineno); up->rcolset=1; } else if(strcmp(name, "ncol")==0) { if(up->ncolset) continue; gal_checkset_sizet_el_zero(value, &p->ncol, name, key, SPACK, filename, lineno); up->ncolset=1; } else if(strcmp(name, "pcol")==0) { if(up->pcolset) continue; gal_checkset_sizet_el_zero(value, &p->pcol, name, key, SPACK, filename, lineno); up->pcolset=1; } else if(strcmp(name, "qcol")==0) { if(up->qcolset) continue; gal_checkset_sizet_el_zero(value, &p->qcol, name, key, SPACK, filename, lineno); up->qcolset=1; } else if(strcmp(name, "mcol")==0) { if(up->mcolset) continue; gal_checkset_sizet_el_zero(value, &p->mcol, name, key, SPACK, filename, lineno); up->mcolset=1; } else if(strcmp(name, "tcol")==0) { if(up->tcolset) continue; gal_checkset_sizet_el_zero(value, &p->tcol, name, key, SPACK, filename, lineno); up->tcolset=1; } else if(strcmp(name, "mforflatpix")==0) { if(up->mforflatpixset) continue; gal_checkset_int_zero_or_one(value, &p->mforflatpix, name, key, SPACK, filename, lineno); up->mforflatpixset=1; } /* WCS: */ else if(strcmp(name, "crpix1")==0) { if(up->crpix1set) continue; gal_checkset_any_double(value, &p->crpix[0], name, key, SPACK, filename, lineno); up->crpix1set=1; } else if(strcmp(name, "crpix2")==0) { if(up->crpix2set) continue; gal_checkset_any_double(value, &p->crpix[1], name, key, SPACK, filename, lineno); up->crpix2set=1; } else if(strcmp(name, "crval1")==0) { if(up->crval1set) continue; gal_checkset_any_double(value, &p->crval[0], name, key, SPACK, filename, lineno); up->crval1set=1; } else if(strcmp(name, "crval2")==0) { if(up->crval2set) continue; gal_checkset_any_double(value, &p->crval[1], name, key, SPACK, filename, lineno); up->crval2set=1; } else if(strcmp(name, "resolution")==0) { if(up->resolutionset) continue; gal_checkset_any_float(value, &p->resolution, name, key, SPACK, filename, lineno); up->resolutionset=1; } /* Operating modes: */ /* Read options common to all programs */ GAL_CONFIGFILES_READ_COMMONOPTIONS_FROM_CONF else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s` not recognized.\n", name); } free(line); fclose(fp); } void printvalues(FILE *fp, struct mkprofparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; fprintf(fp, "\n# Input:\n"); if(cp->hduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("hdu", cp->hdu); fprintf(fp, "\n# Output:\n"); if(cp->outputset) fprintf(fp, CONF_SHOWFMT"%s\n", "output", cp->output); if(up->naxis1set) fprintf(fp, CONF_SHOWFMT"%zu\n", "naxis1", p->naxes[0]); if(up->naxis2set) fprintf(fp, CONF_SHOWFMT"%zu\n", "naxis2", p->naxes[1]); if(up->inputascanvasset) fprintf(fp, CONF_SHOWFMT"%d\n", "inputascanvas", up->inputascanvas); if(up->oversampleset) fprintf(fp, CONF_SHOWFMT"%zu\n", "oversample", p->oversample); if(up->replaceset) fprintf(fp, CONF_SHOWFMT"%d\n", "replace", p->replace); if(up->typeset) gal_configfiles_print_type(fp, p->up.type); fprintf(fp, "\n# Profiles:\n"); if(up->tunitinpset) fprintf(fp, CONF_SHOWFMT"%d\n", "tunitinp", p->tunitinp); if(up->numrandomset) fprintf(fp, CONF_SHOWFMT"%zu\n", "numrandom", p->numrandom); if(up->toleranceset) fprintf(fp, CONF_SHOWFMT"%.2f\n", "tolerance", p->tolerance); if(up->zeropointset) fprintf(fp, CONF_SHOWFMT"%.2f\n", "zeropoint", p->zeropoint); if(up->circumwidthset) fprintf(fp, CONF_SHOWFMT"%.2f\n", "circumwidth", p->circumwidth); if(up->envseedset) fprintf(fp, CONF_SHOWFMT"%d\n", "envseed", p->envseed); fprintf(fp, "\n# Catalog:\n"); if(up->xcolset) fprintf(fp, CONF_SHOWFMT"%zu\n", "xcol", p->xcol); if(up->ycolset) fprintf(fp, CONF_SHOWFMT"%zu\n", "ycol", p->ycol); if(up->racolset) fprintf(fp, CONF_SHOWFMT"%zu\n", "racol", p->racol); if(up->deccolset) fprintf(fp, CONF_SHOWFMT"%zu\n", "deccol", p->deccol); if(up->fcolset) fprintf(fp, CONF_SHOWFMT"%zu\n", "fcol", p->fcol); if(up->rcolset) fprintf(fp, CONF_SHOWFMT"%zu\n", "rcol", p->rcol); if(up->ncolset) fprintf(fp, CONF_SHOWFMT"%zu\n", "ncol", p->ncol); if(up->pcolset) fprintf(fp, CONF_SHOWFMT"%zu\n", "pcol", p->pcol); if(up->qcolset) fprintf(fp, CONF_SHOWFMT"%zu\n", "qcol", p->qcol); if(up->mcolset) fprintf(fp, CONF_SHOWFMT"%zu\n", "mcol", p->mcol); if(up->tcolset) fprintf(fp, CONF_SHOWFMT"%zu\n", "tcol", p->tcol); if(up->mforflatpixset) fprintf(fp, CONF_SHOWFMT"%d\n", "mforflatpix", p->mforflatpix); fprintf(fp, "\n# WCS:\n"); if(up->crpix1set) fprintf(fp, CONF_SHOWFMT"%g\n", "crpix1", p->crpix[0]); if(up->crpix2set) fprintf(fp, CONF_SHOWFMT"%g\n", "crpix2", p->crpix[1]); if(up->crval1set) fprintf(fp, CONF_SHOWFMT"%g\n", "crval1", p->crval[0]); if(up->crval2set) fprintf(fp, CONF_SHOWFMT"%g\n", "crval2", p->crval[1]); if(up->resolutionset) fprintf(fp, CONF_SHOWFMT"%g\n", "resolution", p->resolution); /* For the operating mode, first put the macro to print the common options, then the (possible options particular to this program). */ fprintf(fp, "\n# Operating modes:\n"); GAL_CONFIGFILES_PRINT_COMMONOPTIONS; } void checkifset(struct mkprofparams *p) { struct uiparams *up=&p->up; int intro=0; if(p->cp.hduset==0) GAL_CONFIGFILES_REPORT_NOTSET("hdu"); if(up->tunitinpset==0) GAL_CONFIGFILES_REPORT_NOTSET("tunitinp"); if(up->numrandomset==0) GAL_CONFIGFILES_REPORT_NOTSET("numrandom"); if(up->toleranceset==0) GAL_CONFIGFILES_REPORT_NOTSET("tolerance"); if(up->zeropointset==0) GAL_CONFIGFILES_REPORT_NOTSET("zeropoint"); if(up->fcolset==0) GAL_CONFIGFILES_REPORT_NOTSET("fcol"); if(up->rcolset==0) GAL_CONFIGFILES_REPORT_NOTSET("rcol"); if(up->ncolset==0) GAL_CONFIGFILES_REPORT_NOTSET("ncol"); if(up->pcolset==0) GAL_CONFIGFILES_REPORT_NOTSET("pcol"); if(up->qcolset==0) GAL_CONFIGFILES_REPORT_NOTSET("qcol"); if(up->mcolset==0) GAL_CONFIGFILES_REPORT_NOTSET("mcol"); if(up->oversampleset==0) GAL_CONFIGFILES_REPORT_NOTSET("oversample"); if(up->circumwidthset==0) GAL_CONFIGFILES_REPORT_NOTSET("circumwidth"); /* The output image size, type, and WCS are only necessary if the user has not provided an input image. */ if(p->up.backname==NULL) { if(up->typeset==0) GAL_CONFIGFILES_REPORT_NOTSET("type"); if(up->naxis1set==0) GAL_CONFIGFILES_REPORT_NOTSET("naxis1"); if(up->naxis2set==0) GAL_CONFIGFILES_REPORT_NOTSET("naxis2"); if(up->crpix1set==0) GAL_CONFIGFILES_REPORT_NOTSET("crpix1"); if(up->crpix2set==0) GAL_CONFIGFILES_REPORT_NOTSET("crpix2"); if(up->crval1set==0) GAL_CONFIGFILES_REPORT_NOTSET("crval1"); if(up->crval2set==0) GAL_CONFIGFILES_REPORT_NOTSET("crval2"); if(up->resolutionset==0) GAL_CONFIGFILES_REPORT_NOTSET("resolution"); } /* The X and Y columns are only needed when the RA and Dec columns have not been given. */ if(up->racolset==0 && up->deccolset==0) { if(up->xcolset==0) GAL_CONFIGFILES_REPORT_NOTSET("xcol"); if(up->ycolset==0) GAL_CONFIGFILES_REPORT_NOTSET("ycol"); } /* The `if' statment above made sure that at least one of the RA and Dec columns have been specified. So make sure that both are specified. */ else if(up->racolset!=up->deccolset) { if(up->racolset==0) GAL_CONFIGFILES_REPORT_NOTSET("racol"); if(up->deccolset==0) GAL_CONFIGFILES_REPORT_NOTSET("deccol"); } GAL_CONFIGFILES_END_OF_NOTSET_REPORT; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ void sanitycheck(struct mkprofparams *p) { int d0f1; long width[2]={1,1}; struct uiparams *up=&p->up; double truncr, *cat=p->cat, *row; size_t i, j, columns[9], cs1=p->cs1; char *tmpname=NULL, *xcolstr, *ycolstr; /* Check if over-sampling is an odd number, then set/modify the respective values.*/ if(p->oversample%2==0) error(EXIT_FAILURE, 0, "the value to the `--oversample' (`-s') option " "must be an odd number. Please run the following command for a " "complete explanation:\n\n info gnuastro \"Oversampling\"\n\nOr " "See the \"Oversampling\" section of the Gnuastro book."); p->halfpixel = 0.5f/p->oversample; p->naxes[0] *= p->oversample; p->naxes[1] *= p->oversample; /* When the RA and Dec columns have been given use them for the profile positions instead of the X and Y columns. In the next step we are going to convert the RAs and Decs to Xs and Ys and until then, we are just dealing with the columns, not the actual values, so it is safe (and greatfly simplifies the sanity checks below) to set xcol to ra column and ycol to deccol. Also use this check to set the string that should be printed if the column is not within the catalog's number of columsn*/ if(up->racolset) { p->xcol=p->racol; p->ycol=p->deccol; xcolstr="racol"; ycolstr="deccol"; } else { xcolstr="xcol"; ycolstr="ycol"; } /* If the column numbers are not equal. */ columns[0]=p->xcol; columns[1]=p->ycol; columns[2]=p->fcol; columns[3]=p->rcol; columns[4]=p->ncol; columns[5]=p->pcol; columns[6]=p->qcol; columns[7]=p->mcol; columns[8]=p->tcol; for(i=0;i<9;++i) for(j=0;j<9;++j) if(i!=j && columns[i]==columns[j]) error(EXIT_FAILURE, 0, "at least two of the specified columns " "are set to %zu! By adding the `-P` or `--printparams` " "option you can check the final column numbers. They " "all have to be different", columns[i]); /* If all the columns are within the catalog and have proper values. */ GAL_CHECKSET_CHECK_COL_IN_CAT(p->xcol, xcolstr); GAL_CHECKSET_CHECK_COL_IN_CAT(p->ycol, ycolstr); GAL_CHECKSET_CHECK_COL_IN_CAT(p->fcol, "fcol"); GAL_CHECKSET_CHECK_COL_IN_CAT(p->rcol, "rcol"); GAL_CHECKSET_CHECK_COL_IN_CAT(p->ncol, "ncol"); GAL_CHECKSET_CHECK_COL_IN_CAT(p->pcol, "pcol"); GAL_CHECKSET_CHECK_COL_IN_CAT(p->qcol, "qcol"); GAL_CHECKSET_CHECK_COL_NUM_IN_CAT(p->mcol, "mcol"); GAL_CHECKSET_CHECK_COL_IN_CAT(p->tcol, "tcol"); /* If there were terms that gal_txtarray_txt_to_array could not read, delete the log file. Note that don't care about the whole input catalog, we just want the columns that are important to MakeProfiles. The GAL_CHECKSET_CHECK_COL_IN_CAT tests above checked those columns and they are fine. For example the user might have some alphabetic information in the input file, but as long as the columns we want are correct, we have no problem. We can't remove this line before those tests, because in their errors, those tests guide the reader to check the `txtarray.log' file. */ gal_checkset_check_remove_file(GAL_TXTARRAY_LOG, 0); /* Check if all the profile codes are within the desired range: */ for(i=0;ics0;++i) if(cat[i*cs1+p->fcol]<0 || cat[i*cs1+p->fcol]>MAXIMUMCODE) error(EXIT_FAILURE, 0, "%s: In row %zu, the function code should" "be positive and smaller or equal to %d", p->up.catname, i+1, MAXIMUMCODE); /* If any of xshift or yshift is non-zero, the other should be too! Note that conditional operators return 1 if true and 0 if false, so if one is non-zero while the other is zero, then sum will be 1. Otherwise the sum will either be 0 or 2.*/ switch ( (p->shift[0]!=0) + (p->shift[1]!=0) ) { /* If prepforconv is called, then xshift and yshift should be zero. Also a Moffat or Gaussian profile should exist in the image. */ case 0: if(p->up.prepforconv) { /* Check if there is at least one Moffat or Gaussian profile. */ j=0; for(i=0;ics0;++i) if(ispsf(cat[i*cs1+p->fcol])) { j=i; break; } /* If there is no PSF in the catalog, then you can ignore prepforconv. */ if(ics0) { /* Set the row, to simplify: */ row=&cat[j*cs1]; /* Find the correct xshift and yshift using the first Moffat or Gaussian profile (in row 'j'). Note that the output of encloseellipse will be the total width, we only want half of it for the shift.*/ truncr = ( p->tunitinp ? row[p->tcol] : row[p->tcol] * row[p->rcol]/2); gal_box_ellipse_in_box(truncr, row[p->qcol]*truncr, row[p->pcol]*DEGREESTORADIANS, width); p->shift[0] = (width[0]/2)*p->oversample; p->shift[1] = (width[1]/2)*p->oversample; } } break; case 1: error(EXIT_FAILURE, 0, "at least one of `--xshift` (`-X`) or " "`--yshift` (`-Y`) are zero"); break; case 2: p->shift[0] *= p->oversample; p->shift[1] *= p->oversample; break; default: error(EXIT_FAILURE, 0, "a bug in sanitycheck (ui.c)! In checks " "for shifts. Please contact us so we can fix it"); } p->naxes[0] += 2*p->shift[0]; p->naxes[1] += 2*p->shift[1]; /* Check the output name: */ d0f1=gal_checkset_dir_0_file_1(p->cp.output, p->cp.dontdelete); if(d0f1) /* --output is a file name. */ { p->mergedimgname=p->cp.output; p->outdir=gal_checkset_dir_part(p->mergedimgname); } else /* --output is a directory name. */ { errno=0; p->outdir=malloc((strlen(p->cp.output)+1)*sizeof *p->outdir); if(p->outdir==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->outdir in ui.c", (strlen(p->cp.output)+1)*sizeof *p->outdir); strcpy(p->outdir, p->cp.output); gal_checkset_check_dir_write_add_slash(&p->outdir); gal_checkset_automatic_output(p->up.catname, ".fits", p->cp.removedirinfo, p->cp.dontdelete, &tmpname); p->mergedimgname=gal_checkset_malloc_cat(p->outdir, tmpname); free(tmpname); } p->basename=gal_checkset_not_dir_part(p->mergedimgname); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ void preparewcs(struct mkprofparams *p) { int status; struct wcsprm *wcs; long os=p->oversample; /* Allocate the memory necessary for the wcsprm structure. */ errno=0; wcs=p->wcs=malloc(sizeof *wcs); if(wcs==NULL) error(EXIT_FAILURE, errno, "%zu for wcs in preparewcs", sizeof *wcs); /* Initialize the structure (allocate all the arrays). */ wcs->flag=-1; if( (status=wcsini(1, 2, wcs)) ) error(EXIT_FAILURE, 0, "wcsinit error %d: %s", status, wcs_errmsg[status]); /* Correct the CRPIX values based on oversampling and shifting. */ p->crpix[0] = p->crpix[0]*os + p->shift[0] - os/2; p->crpix[1] = p->crpix[1]*os + p->shift[1] - os/2; /* Fill in all the important WCS structure parameters. */ wcs->equinox=2000.0f; wcs->crpix[0]=p->crpix[0]; wcs->crpix[1]=p->crpix[1]; wcs->crval[0]=p->crval[0]; wcs->crval[1]=p->crval[1]; wcs->pc[0]=-1.0f*p->resolution/3600/p->oversample; wcs->pc[3]=p->resolution/3600/p->oversample; wcs->pc[1]=wcs->pc[2]=0.0f; wcs->cdelt[0]=wcs->cdelt[1]=1.0f; strcpy(wcs->cunit[0], "deg"); strcpy(wcs->cunit[1], "deg"); strcpy(wcs->ctype[0], "RA---TAN"); strcpy(wcs->ctype[1], "DEC--TAN"); /* Set up the wcs structure with the constants defined above. */ status=wcsset(wcs); if(status) error(EXIT_FAILURE, 0, "wcsset error %d: %s", status, wcs_errmsg[status]); /* When individual mode is requested, write the WCS structure to a header string to speed up the process: if we don't do it here, this process will be necessary on every individual profile's output. */ if(p->individual) { status=wcshdo(WCSHDO_safe, wcs, &p->wcsnkeyrec, &p->wcsheader); if(status) error(EXIT_FAILURE, 0, "wcshdo error %d: %s", status, wcs_errmsg[status]); } } void preparearrays(struct mkprofparams *p) { void *array=NULL; size_t i, naxes[2]; double *wcstoimg=NULL; struct uiparams *up=&p->up; /* Allocate space for the log file: */ p->log=malloc(p->cs0*LOGNUMCOLS*sizeof *p->log); if(p->log==NULL) error(EXIT_FAILURE, 0, "Allocating %zu bytes for log file", p->cs0*LOGNUMCOLS*sizeof *p->log); /* If a background image is specified, then use that as the output image to build the profiles over. */ if(up->backname) { /* Read the input WCS. */ gal_fits_read_wcs(up->backname, p->cp.hdu, 0, 0, &p->nwcs, &p->wcs); /* Read in the background image and its coordinates: */ p->anyblank=gal_fits_hdu_to_array(up->backname, p->cp.hdu, &p->bitpix, &array, &naxes[1], &naxes[0]); p->naxes[1]=naxes[1]; p->naxes[0]=naxes[0]; /* The the type of the input image is not float, then convert it to float to add the mock profile. */ if(p->bitpix==FLOAT_IMG) p->out=array; else { gal_fits_change_type(array, p->bitpix, p->naxes[1]*p->naxes[0], p->anyblank, (void **)(&p->out), FLOAT_IMG); free(array); } /* If the user just wanted the headers, then change all non-NaN pixels to 0.0f. */ if(up->inputascanvas) gal_array_freplace_nonnans(p->out, naxes[0]*naxes[1], 0.0f); } /* Make the WCS structure if it has not been set so far. */ if(p->wcs==NULL) preparewcs(p); /* Set the output image type when a background image is not specified, or when inputascanvas is called (with a background image). */ if(!up->backname || up->inputascanvas) p->bitpix=up->type; /* Convert the RA and Dec to X and Y. We will make a temporary array with four rows and the same number of columns, then use that array and the WCS structure to get X and Y values. Those X and Y values will then be replaced with the RAs and Decs of the original catalog. Recall that this is only done in the RAM, not the actual input file, so there is no problem. One of the reasons we are doing this is that WCSLIB needs the X and Ys and the RA and Decs to be in touching pieces of memory and we can't guarantee that (the user might have these columns in any order). */ if(up->racolset) { /* Allocate the space for the temporary array. */ errno=0; wcstoimg=malloc(4*p->cs0*sizeof *wcstoimg); if(wcstoimg==NULL) error(EXIT_FAILURE, errno, "%zu bytes for wcstoimg", 4*p->cs0*sizeof *wcstoimg); /* Fill in the first two columns with the RA and Dec. */ for(i=0;ics0;++i) { wcstoimg[ i*4 ] = p->cat[ i*p->cs1+p->racol ]; wcstoimg[ i*4+1 ] = p->cat[ i*p->cs1+p->deccol ]; wcstoimg[ i*4+2 ] = wcstoimg[ i*4+3 ] = NAN; } /* Convert the X and Y to RA and Dec. */ gal_wcs_radec_array_to_xy(p->wcs, wcstoimg, wcstoimg+2, p->cs0, 4); /* Write the produced X and Y into the input catalog, note that in `sanitycheck', xcol became identical to racol and ycol to deccol. Note that oversampling has been applied to the WCS structure. However, when X and Y are given, oversampling is not applied at this point, so we have to correct for the WCS's oversampling.*/ for(i=0;ics0;++i) { p->cat[ i*p->cs1+p->xcol ] = wcstoimg[ i*4+2 ] / p->oversample; p->cat[ i*p->cs1+p->ycol ] = wcstoimg[ i*4+3 ] / p->oversample; } /* Free the temporary array space. */ free(wcstoimg); } /* Allocate the random number generator: */ gsl_rng_env_setup(); p->rng=gsl_rng_alloc(gsl_rng_default); } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void setparams(int argc, char *argv[], struct mkprofparams *p) { char *jobname; struct timeval t1; struct gal_commonparams *cp=&p->cp; char message[GAL_TIMING_VERB_MSG_LENGTH_V]; /* Set the non-zero initial values, the structure was initialized to have a zero value for all elements. */ cp->spack = SPACK; cp->verb = 1; cp->numthreads = num_processors(NPROC_CURRENT); cp->removedirinfo = 1; p->out = NULL; p->wcs = NULL; p->mforflatpix = 0; p->up.inputascanvas = 0; /* Read the arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Add the user default values and save them if asked. */ GAL_CONFIGFILES_CHECK_SET_CONFIG; /* Check if all the required parameters are set. */ checkifset(p); /* Print the values for each parameter. */ if(cp->printparams) GAL_CONFIGFILES_REPORT_PARAMETERS_SET; /* Read catalog if given. */ gal_txtarray_txt_to_array(p->up.catname, &p->cat, &p->cs0, &p->cs1); /* If cp->output was not specified on the command line or in any of the configuration files, then automatic output should be used, in which case, cp->output should be the current directory. */ if(p->cp.outputset==0) { gal_checkset_allocate_copy("./", &p->cp.output); p->cp.outputset=1; } /* Do a sanity check, then remove the possibly existing log file created by gal_txtarray_txt_to_array. */ gettimeofday(&t1, NULL); sanitycheck(p); /* Prepare the necessary arrays: */ preparearrays(p); /* Everything is ready, notify the user of the program starting. */ if(cp->verb) { printf(SPACK_NAME" started on %s", ctime(&p->rawtime)); errno=0; jobname=malloc(strlen(p->up.catname)+100*sizeof *jobname); if(jobname==NULL) error(EXIT_FAILURE, errno, "jobname in ui.c"); sprintf(jobname, "%zu profile%sread from %s", p->cs0, p->cs0>1?"s ":" ", p->up.catname); gal_timing_report(&t1, jobname, 1); free(jobname); sprintf(message, "Random number generator (RNG) type: %s", gsl_rng_name(p->rng)); gal_timing_report(NULL, message, 1); if(p->envseed) { sprintf(message, "RNG seed for all profiles: %zu", gsl_rng_default_seed); gal_timing_report(NULL, message, 1); } sprintf(message, "Using %zu threads.", cp->numthreads); gal_timing_report(NULL, message, 1); } } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void freeandreport(struct mkprofparams *p, struct timeval *t1) { int status; /* Free all the allocated arrays. */ free(p->cat); free(p->cp.hdu); free(p->outdir); free(p->basename); if(p->individual==0) free(p->log); /* p->cp.output might be equal to p->mergedimgname. In this case, if we simply free them after each other, there will be a double free error. So after freeing output, we set it to NULL since free(NULL) is ok.*/ if(p->cp.output==p->mergedimgname) free(p->cp.output); else { free(p->cp.output); free(p->mergedimgname); } /* Free the WCS headers string that was defined for individual mode. */ if(p->individual) free(p->wcsheader); /* Free the WCS structure. */ if( (status=wcsvfree(&p->nwcs, &p->wcs)) ) error(EXIT_FAILURE, 0, "wcsfree error %d: %s", status, wcs_errmsg[status]); /* Free the random number generator: */ gsl_rng_free(p->rng); /* Print the final message. */ if(p->cp.verb) gal_timing_report(t1, SPACK_NAME" finished in: ", 0); } gnuastro-0.2.33-8a3b/bin/mkprof/main.h0000644000175000017500000002045312774157746014310 00000000000000/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include #include #include #include /* Progarm name macros: */ #define SPACK "astmkprof" /* Subpackage executable name. */ #define SPACK_NAME "MakeProfiles" /* Subpackage full name. */ #define SPACK_STRING SPACK_NAME" ("PACKAGE_NAME") "PACKAGE_VERSION #define LOGFILENAME SPACK".log" #define LOGNUMCOLS 5 #define DEGREESTORADIANS M_PI/180.0f #define SERSICCODE 0 #define MOFFATCODE 1 #define GAUSSIANCODE 2 #define POINTCODE 3 #define FLATCODE 4 #define CIRCUMFERENCECODE 5 #define MAXIMUMCODE 5 #define EPSREL_FOR_INTEG 2 #define MINCIRCUMWIDTH 0.5f /* Log columns: 0: ID. 1: Overlap magnitude. 2: Number of accurate pixels. 3: Fraction of accurate values. 4: Is individual file created? */ struct builtqueue { size_t id; /* ID of this object. */ int ispsf; /* This is a PSF profile. */ int overlaps; /* ==1: Overlaps with the image. */ float *img; /* Array of this profile's image. */ size_t imgwidth; /* Width of *img. */ long fpixel_i[2]; /* First pixel in output image. */ long lpixel_i[2]; /* Last pixel in output image. */ long fpixel_o[2]; /* First pixel in this array. */ int type; /* The type of the profile. */ int indivcreated; /* ==1: an individual file is created. */ size_t numaccu; /* Number of accurate pixels. */ double accufrac; /* Difference of accurate values. */ struct builtqueue *next; /* Pointer to next element. */ }; struct uiparams { int type; /* User's desired output bitpix. */ char *backname; /* Name of background image file name. */ char *backhdu; /* HDU of background image. */ char *catname; /* Name of catalog of parameters. */ int prepforconv; /* Shift and expand by size of first psf. */ int inputascanvas; /* Input image's header for size and WCS. */ /* Check if all parameters are read (use .def file for comparison). The non optional parameters (like the catalog and input FITS images that come in from arguments, not options) are checked in the args.h files. */ int backhduset; int naxis1set; int naxis2set; int oversampleset; int circumwidthset; int envseedset; int replaceset; int typeset; int inputascanvasset; int tunitinpset; int numrandomset; int toleranceset; int zeropointset; int xshiftset; int yshiftset; int prepforconvset; int fcolset; int xcolset; int ycolset; int racolset; int deccolset; int rcolset; int ncolset; int pcolset; int qcolset; int mcolset; int tcolset; int mforflatpixset; int crpix1set; int crpix2set; int crval1set; int crval2set; int resolutionset; }; struct mkprofparams { /* Other structures */ struct uiparams up; /* User interface parameters. */ struct gal_commonparams cp; /* Common parameters. */ /* Operating modes */ int psfinimg; /* ==1: Build PSF profiles in image. */ int individual; /* ==1: Build all catalog separately. */ /* Profiles */ int replace; /* Replace overlaping profile pixel values. */ size_t numrandom; /* Number of radom points for integration. */ float tolerance; /* Accuracy to stop integration. */ float zeropoint; /* Magnitude of zero point flux. */ double circumwidth; /* Width of circumference (inward). */ int magatpeak; /* Mag only for peak pixel, not all profile.*/ int envseed; /* Use GSL_RNG_SEED for random seed. */ int tunitinp; /* ==1: Truncation unit is in pixels. */ /* ==0: It is in radial parameter. */ /* Catalog */ size_t fcol; /* Column specifying profile function. */ size_t xcol; /* X column of profile center. */ size_t ycol; /* Y column of profile center. */ size_t racol; /* RA column of profile center. */ size_t deccol; /* Dec column of profile center. */ size_t rcol; /* Effective radius of profile. */ size_t ncol; /* Sersic index column of profile. */ size_t pcol; /* Position angle column of profile. */ size_t qcol; /* Axis ratio column of profile. */ size_t mcol; /* Magnitude column. */ size_t tcol; /* Truncation of the profiles. */ int mforflatpix; /* mcol is flat pixel value (f is 4 or 5). */ /* Random number generator */ gsl_rng *rng; /* Main instance of random number generator.*/ /* Output */ char *basename; /* Merged image name with no directory. */ char *outdir; /* Output directory. */ int anyblank; /* ==1: there are blanks in back. */ int bitpix; /* bitpix of backgroud/output image. */ int nomerged; /* ==1: Don't make a merged image of all. */ long naxes[2]; /* Size of the output image. */ long shift[2]; /* Shift along axeses position of profiles. */ size_t oversample; /* Oversampling scale. */ int nwcs; /* Number of WCS. */ struct wcsprm *wcs; /* WCSparam structure. */ /* WCS: */ double crpix[2]; /* CRPIX FITS header keywords. */ double crval[2]; /* CRVAL FITS header keywords. */ float resolution; /* PC1_1 and PC2_2 FITS header keywords. */ /* Internal parameters: */ time_t rawtime; /* Starting time of the program. */ float *out; /* Output image. */ double *cat; /* Input catalog. */ size_t cs0; /* Number of rows in input catalog. */ size_t cs1; /* Number of columns in input catalog. */ double *log; /* Log data to be printed. */ struct builtqueue *bq; /* Top (last) elem of build queue. */ pthread_cond_t qready; /* bq is ready to be written. */ pthread_mutex_t qlock; /* Mutex lock to change builtq. */ double halfpixel; /* Half pixel in oversampled image. */ char *wcsheader; /* The WCS header information for main img. */ int wcsnkeyrec; /* The number of keywords in the WCS header.*/ char *mergedimgname; /* Name of merged image. */ }; #endif gnuastro-0.2.33-8a3b/bin/mkprof/main.c0000644000175000017500000000314412774157611014270 00000000000000/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include /* Includes time.h and sys/time.h */ #include "main.h" #include "mkprof.h" #include "ui.h" /* needs main.h. */ int main (int argc, char *argv[]) { struct timeval t1; struct mkprofparams p={{0}, {0}, 0}; /* Set the starting time.*/ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ setparams(argc, argv, &p); /* Run MakeProfiles */ mkprof(&p); /* Free all non-freed allocations. */ freeandreport(&p, &t1); /* Return successfully.*/ return EXIT_SUCCESS; } gnuastro-0.2.33-8a3b/bin/mkprof/Makefile.in0000644000175000017500000017305613004464627015252 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without 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GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = 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This file is offered as-is, # without any warranty. # Input: hdu 0 # Output: naxis1 1000 naxis2 1000 oversample 5 circumwidth 2 type float # Profiles: tunitinp 0 numrandom 10000 tolerance 0.01 zeropoint 0.00 prepforconv 0 xshift 0 yshift 0 # Catalog: xcol 1 ycol 2 fcol 3 rcol 4 ncol 5 pcol 6 qcol 7 mcol 8 tcol 9 # WCS: crpix1 1 crpix2 1 crval1 1 crval2 1 resolution 0.03gnuastro-0.2.33-8a3b/bin/mkprof/Makefile.am0000644000175000017500000000276312765246730015243 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. NOTE: $(top_srcdir)/bootstrapped/lib is only necessary ## for internally compiled utilities and libraries. It must not be included ## during the tests since the bootstrapped libraries are not installed. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib # Utility and its sources bin_PROGRAMS = astmkprof astmkprof_SOURCES = main.c main.h ui.c ui.h mkprof.c mkprof.h args.h \ oneprofile.c oneprofile.h profiles.c profiles.h cite.h astmkprof_LDADD = $(top_builddir)/bootstrapped/lib/libgnu.la \ -lgnuastro ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astmkprof.conf gnuastro-0.2.33-8a3b/bin/mknoise/0000755000175000017500000000000013004464725013417 500000000000000gnuastro-0.2.33-8a3b/bin/mknoise/mknoise.h0000644000175000017500000000204712616616510015157 00000000000000/********************************************************************* MakeNoise - Add noise to a dataset. MakeNoise is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MKNOISE_H #define MKNOISE_H void mknoise(struct mknoiseparams *p); #endif gnuastro-0.2.33-8a3b/bin/mknoise/mknoise.c0000644000175000017500000000730112774157570015163 00000000000000/********************************************************************* MakeNoise - Add noise to a dataset. MakeNoise is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* Generate random seed. */ #include /* Used in setrandoms. */ #include #include /* To make noise. */ #include #include "main.h" void convertsaveoutput(struct mknoiseparams *p) { void *array; char keyname1[FLEN_KEYWORD]; struct gal_fits_key_ll *headers=NULL; char keyname2[FLEN_KEYWORD], keyname3[FLEN_KEYWORD]; char keyname4[FLEN_KEYWORD], keyname5[FLEN_KEYWORD]; /* Convert the output to the input image format: */ if(p->inputbitpix==DOUBLE_IMG || p->doubletype) { array=p->input; p->inputbitpix=DOUBLE_IMG; /* Not converted and p->doubletype==1 */ } else gal_fits_change_type((void **)p->input, DOUBLE_IMG, p->is0*p->is1, p->anyblank, &array, p->inputbitpix); /* Add the proper information to the header of the output: */ gal_fits_file_name_in_keywords("INF", p->up.inputname, &headers); strcpy(keyname1, "BCKGRND"); gal_fits_add_to_key_ll_end(&headers, TDOUBLE, keyname1, 0, &p->mbackground, 0, "Background " "value (in magnitude) for noise.", 0, NULL); strcpy(keyname2, "BZRPNT"); gal_fits_add_to_key_ll_end(&headers, TDOUBLE, keyname2, 0, &p->zeropoint, 0, "Zeropoint magnitude of image.", 0, NULL); strcpy(keyname3, "STDADD"); gal_fits_add_to_key_ll_end(&headers, TDOUBLE, keyname3, 0, &p->stdadd, 0, "Instrumental noise in units of flux.", 0, NULL); strcpy(keyname4, "RNGTYPE"); gal_fits_add_to_key_ll_end(&headers, TSTRING, keyname4, 0, &p->rng_type, 0, "Random number generator (by GSL) type.", 0, NULL); strcpy(keyname5, "RNGSEED"); gal_fits_add_to_key_ll_end(&headers, TLONG, keyname5, 0, &p->rng_seed, 0, "Random number generator (by GSL) seed.", 0, NULL); /* Save the output: */ gal_fits_array_to_file(p->cp.output, "NoiseAdded", p->inputbitpix, array, p->is0, p->is1, p->anyblank, p->wcs, headers, SPACK_STRING); if(array!=p->input) free(array); } void mknoise(struct mknoiseparams *p) { double *d, *df, background=p->background, stdadd=p->stdadd; /* Add the noise: */ df=(d=p->input)+p->is0*p->is1; do *d+=background+gsl_ran_gaussian(p->rng, sqrt(stdadd+background+*d)); while(++d Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef ARGS_H #define ARGS_H #include #include #include /**************************************************************/ /************** argp.h definitions ***************/ /**************************************************************/ /* Definition parameters for the argp: */ const char *argp_program_version=SPACK_STRING"\n"GAL_STRINGS_COPYRIGHT "\n\nWritten by Mohammad Akhlaghi"; const char *argp_program_bug_address=PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata ..."; const char doc[] = /* Before the list of options: */ GAL_STRINGS_TOP_HELP_INFO SPACK_NAME" will add noise to all the pixels in an input image. The noise " "parameters can be specified with the command line options. \n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /* Available letters for short options: a c f g i j k l m n p r t u v w x y A B C E F G H I J L M O Q R T U W X Y Z Number keys used: Nothing! Options with keys (second structure element) larger than 500 do not have a short version. */ static struct argp_option options[] = { { 0, 0, 0, 0, "Input:", 1 }, { "stdadd", 's', "FLT", 0, "Standard deviation addition constant.", 1 }, { "background", 'b', "FLT", 0, "Fixed background magnitude for the image.", 1 }, { "zeropoint", 'z', "FLT", 0, "Image zeropoint magnitude.", 1 }, { "envseed", 'e', 0, 0, "Use GSL_RNG_SEED environment variable for seed.", 1 }, { 0, 0, 0, 0, "Output:", 2 }, { "doubletype", 'd', 0, 0, "Save output as a double precision floating point.", 2 }, { 0, 0, 0, 0, "Operating modes:", -1 }, {0} }; /* Parse a single option: */ static error_t parse_opt(int key, char *arg, struct argp_state *state) { /* Save the arguments structure: */ struct mknoiseparams *p = state->input; /* Set the pointer to the common parameters for all programs here: */ state->child_inputs[0]=&p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); switch(key) { /* Input: */ case 'b': gal_checkset_any_double(arg, &p->mbackground, "background", key, SPACK, NULL, 0); p->up.backgroundset=1; break; case 's': gal_checkset_double_el_0(arg, &p->stdadd, "stdadd", key, SPACK, NULL, 0); p->up.stdaddset=1; break; case 'z': gal_checkset_any_double(arg, &p->zeropoint, "zeropoint", key, SPACK, NULL, 0); p->up.zeropointset=1; break; case 'e': p->envseed=1; p->up.envseedset=1; break; /* Output: */ case 'd': p->doubletype=1; break; /* Read the non-option arguments: */ case ARGP_KEY_ARG: /* See what type of input value it is and put it in. */ if( gal_fits_name_is_fits(arg) ) { if(p->up.inputname) argp_error(state, "only one input image should be given"); else p->up.inputname=arg; } else argp_error(state, "%s is not a valid file type", arg); break; /* The command line options and arguments are finished. */ case ARGP_KEY_END: if(p->cp.setdirconf==0 && p->cp.setusrconf==0 && p->cp.printparams==0) { if(state->arg_num==0) argp_error(state, "no argument given"); if(p->up.inputname==NULL) argp_error(state, "no input FITS image(s) provided"); } break; default: return ARGP_ERR_UNKNOWN; } return 0; } /* Specify the children parsers: */ struct argp_child children[]= { {&commonargp, 0, NULL, 0}, {0, 0, 0, 0} }; /* Basic structure defining the whole argument reading process. */ static struct argp thisargp = {options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif gnuastro-0.2.33-8a3b/bin/mknoise/ui.h0000644000175000017500000000220512616616510014123 00000000000000/********************************************************************* MakeNoise - Add noise to a dataset. MakeNoise is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef IMCROPUI_H #define IMCROPUI_H void setparams(int argc, char *argv[], struct mknoiseparams *p); void freeandreport(struct mknoiseparams *p, struct timeval *t1); #endif gnuastro-0.2.33-8a3b/bin/mknoise/ui.c0000644000175000017500000002511213001632540014106 00000000000000/********************************************************************* MakeNoise - Add noise to a dataset. MakeNoise is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include /* From Gnulib. */ #include /* Includes time.h and sys/time.h */ #include #include #include #include "main.h" #include "ui.h" /* Needs main.h */ #include "args.h" /* Needs main.h, includes argp.h. */ /* Set the file names of the places where the default parameters are put. */ #define CONFIG_FILE SPACK CONF_POSTFIX #define SYSCONFIG_FILE SYSCONFIG_DIR "/" CONFIG_FILE #define USERCONFIG_FILEEND USERCONFIG_DIR CONFIG_FILE #define CURDIRCONFIG_FILE CURDIRCONFIG_DIR CONFIG_FILE /**************************************************************/ /************** Options and parameters ***************/ /**************************************************************/ void readconfig(char *filename, struct mknoiseparams *p) { FILE *fp; size_t lineno=0, len=200; char *line, *name, *value; struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; char key='a'; /* Not used, just a place holder. */ /* When the file doesn't exist or can't be opened, it is ignored. It might be intentional, so there is no error. If a parameter is missing, it will be reported after all defaults are read. */ fp=fopen(filename, "r"); if (fp==NULL) return; /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); /* Read the tokens in the file: */ while(getline(&line, &len, fp) != -1) { /* Prepare the "name" and "value" strings, also set lineno. */ GAL_CONFIGFILES_START_READING_LINE; /* Inputs: */ if(strcmp(name, "hdu")==0) gal_checkset_allocate_copy_set(value, &cp->hdu, &cp->hduset); else if(strcmp(name, "background")==0) { if(up->backgroundset) continue; gal_checkset_any_double(value, &p->mbackground, value, key, SPACK, filename, lineno); up->backgroundset=1; } else if(strcmp(name, "zeropoint")==0) { if(up->zeropointset) continue; gal_checkset_any_double(value, &p->zeropoint, value, key, SPACK, filename, lineno); up->zeropointset=1; } else if(strcmp(name, "stdadd")==0) { if(up->stdaddset) continue; gal_checkset_double_el_0(value, &p->stdadd, value, key, SPACK, filename, lineno); up->stdaddset=1; } else if(strcmp(name, "envseed")==0) { if(up->envseedset) continue; gal_checkset_int_zero_or_one(value, &p->envseed, name, key, SPACK, filename, lineno); up->envseedset=1; } /* Outputs */ else if(strcmp(name, "output")==0) gal_checkset_allocate_copy_set(value, &cp->output, &cp->outputset); /* Operating modes: */ /* Read options common to all programs */ GAL_CONFIGFILES_READ_COMMONOPTIONS_FROM_CONF else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s` not recognized.\n", name); } free(line); fclose(fp); } void printvalues(FILE *fp, struct mknoiseparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; /* Print all the options that are set. Separate each group with a commented line explaining the options in that group. */ fprintf(fp, "\n# Input image:\n"); if(cp->hduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("hdu", cp->hdu); if(up->backgroundset) fprintf(fp, CONF_SHOWFMT"%f\n", "background", p->mbackground); if(up->zeropointset) fprintf(fp, CONF_SHOWFMT"%f\n", "zeropoint", p->zeropoint); if(up->stdaddset) fprintf(fp, CONF_SHOWFMT"%f\n", "stdadd", p->stdadd); if(up->envseedset) fprintf(fp, CONF_SHOWFMT"%d\n", "envseed", p->envseed); fprintf(fp, "\n# Output parameters:\n"); if(cp->outputset) fprintf(fp, CONF_SHOWFMT"%s\n", "output", cp->output); /* For the operating mode, first put the macro to print the common options, then the (possible options particular to this program). */ fprintf(fp, "\n# Operating mode:\n"); GAL_CONFIGFILES_PRINT_COMMONOPTIONS; } /* Note that numthreads will be used automatically based on the configure time. */ void checkifset(struct mknoiseparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; int intro=0; if(cp->hduset==0) GAL_CONFIGFILES_REPORT_NOTSET("hdu"); if(up->backgroundset==0) GAL_CONFIGFILES_REPORT_NOTSET("background"); if(up->zeropointset==0) GAL_CONFIGFILES_REPORT_NOTSET("zeropoint"); if(up->stdaddset==0) GAL_CONFIGFILES_REPORT_NOTSET("stdadd"); GAL_CONFIGFILES_END_OF_NOTSET_REPORT; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ void sanitycheck(struct mknoiseparams *p) { /* Make sure the input file exists. */ gal_checkset_check_file(p->up.inputname); /* Set the output name: */ if(p->cp.output) gal_checkset_check_remove_file(p->cp.output, p->cp.dontdelete); else gal_checkset_automatic_output(p->up.inputname, "_noised.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->cp.output); /* Convert the background value from magnitudes to flux. Note that magnitudes are actually calculated from the ratio of brightness, not flux. But in the context of MakeNoise where everything is done on pixels independently, brightness and flux are the same (flux is multiplied by the area of one pixel (=1) to give brightness).*/ p->background=pow(10, (p->zeropoint-p->mbackground)/2.5f); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ void preparearrays(struct mknoiseparams *p) { void *array; /* Read in the input image: */ p->anyblank=gal_fits_hdu_to_array(p->up.inputname, p->cp.hdu, &p->inputbitpix, &array, &p->is0, &p->is1); if(p->inputbitpix==DOUBLE_IMG) p->input=array; else { gal_fits_change_type(array, p->inputbitpix, p->is0*p->is1, p->anyblank, (void **)&p->input, DOUBLE_IMG); free(array); } gal_fits_read_wcs(p->up.inputname, p->cp.hdu, 0, 0, &p->nwcs, &p->wcs); /* Allocate the random number generator: */ gsl_rng_env_setup(); p->rng=gsl_rng_alloc(gsl_rng_default); if(p->envseed==0) gsl_rng_set(p->rng, gal_timing_time_based_rng_seed()); p->rng_seed=gsl_rng_default_seed; strcpy(p->rng_type, gsl_rng_name(p->rng)); } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void setparams(int argc, char *argv[], struct mknoiseparams *p) { char message[GAL_TIMING_VERB_MSG_LENGTH_V]; struct gal_commonparams *cp=&p->cp; /* Set the non-zero initial values, the structure was initialized to have a zero value for all elements. */ cp->spack = SPACK; cp->verb = 1; cp->numthreads = num_processors(NPROC_CURRENT); cp->removedirinfo = 1; /* Read the arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Add the user default values and save them if asked. */ GAL_CONFIGFILES_CHECK_SET_CONFIG; /* Check if all the required parameters are set. */ checkifset(p); /* Print the values for each parameter. */ if(cp->printparams) GAL_CONFIGFILES_REPORT_PARAMETERS_SET; /* Make the array of input images. */ preparearrays(p); /* Do a sanity check. */ sanitycheck(p); /* Everything is ready, notify the user of the program starting. */ if(cp->verb) { printf(SPACK_NAME" started on %s", ctime(&p->rawtime)); sprintf(message, "Random number generator type: %s", gsl_rng_name(p->rng)); gal_timing_report(NULL, message, 1); if(p->envseed) { sprintf(message, "Random number generator seed: %zu", gsl_rng_default_seed); gal_timing_report(NULL, message, 1); } } } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void freeandreport(struct mknoiseparams *p, struct timeval *t1) { /* Free the allocated arrays: */ free(p->input); free(p->cp.hdu); free(p->cp.output); /* The world coordinate system: */ if(p->wcs) wcsvfree(&p->nwcs, &p->wcs); /* Free the random number generator: */ gsl_rng_free(p->rng); /* Print the final message. */ if(p->cp.verb) gal_timing_report(t1, SPACK_NAME" finished in: ", 0); } gnuastro-0.2.33-8a3b/bin/mknoise/cite.h0000644000175000017500000000314612750745735014452 00000000000000/********************************************************************* MakeNoise - Add noise to a dataset. MakeNoise is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CITE_H #define CITE_H #define MKNOISEBIBTEX "" #define PRINTCITEABORT { \ printf("\nWe hope %s has been useful for your research.\n" \ "Citations are vital for the continued work on %s.\n" \ "Thank you for citing it in your research paper.\n" \ "\nPlease cite as \"%s\":\n\n%s\n\n%s", \ SPACK_NAME, SPACK_NAME, SPACK_STRING, \ GAL_STRINGS_MAIN_BIBTEX, MKNOISEBIBTEX); \ exit(EXIT_SUCCESS); \ } #endif gnuastro-0.2.33-8a3b/bin/mknoise/main.h0000644000175000017500000000610012774160636014440 00000000000000/********************************************************************* MakeNoise - Add noise to a dataset. MakeNoise is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include #include #include #include /* Progarm name macros: */ #define SPACK "astmknoise" /* Subpackage executable name. */ #define SPACK_NAME "MakeNoise" /* Subpackage full name. */ #define SPACK_STRING SPACK_NAME" ("PACKAGE_NAME") "PACKAGE_VERSION struct uiparams { char *inputname; /* Name of input file. */ int backgroundset; int zeropointset; int stdaddset; int randseedset; int envseedset; }; struct mknoiseparams { /* Other structures: */ struct uiparams up; /* User interface parameters. */ struct gal_commonparams cp; /* Common parameters. */ /* Input: */ int envseed; /* ==1, generate a random seed. */ double *input; /* Input image data in double precision. */ int inputbitpix; /* Input BITPIX header keyword value. */ size_t is0; /* The number of rows in the input image. */ size_t is1; /* The number of columns in the input image.*/ int anyblank; /* ==1: There are blank pixels in input. */ int nwcs; /* Number of WCS structures. */ struct wcsprm *wcs; /* Pointer to WCS structures. */ double background; /* Mean of noise probability distribution. */ double mbackground; /* Background in magnitudes. */ double stdadd; /* Standard deviation constants. */ double zeropoint; /* Zeropoint magnitude of image. */ /* Random number generator */ gsl_rng *rng; /* Main instance of random number generator.*/ /* Output: */ int doubletype; /* Save the output in double type. */ /* Internal: */ time_t rawtime; /* Starting time of the program. */ char rng_type[FLEN_VALUE]; /* The type of the Random number gen. */ long rng_seed; /* Seed of Random number generator. */ }; #endif gnuastro-0.2.33-8a3b/bin/mknoise/main.c0000644000175000017500000000320612774157467014447 00000000000000/********************************************************************* MakeNoise - Add noise to a dataset. MakeNoise is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include /* Includes time.h and sys/time.h */ #include "main.h" #include "ui.h" /* needs main.h. */ #include "mknoise.h" /* needs main.h. */ int main (int argc, char *argv[]) { struct timeval t1; struct mknoiseparams p={{0}, {0}, 0}; /* Set the starting time.*/ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ setparams(argc, argv, &p); /* Run MakeProfiles */ mknoise(&p); /* Free all non-freed allocations. */ freeandreport(&p, &t1); /* Return successfully.*/ return EXIT_SUCCESS; } gnuastro-0.2.33-8a3b/bin/mknoise/Makefile.in0000644000175000017500000017251713004464627015422 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with 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GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = 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This file is offered as-is, # without any warranty. # Input: hdu 0 background -10.00 stdadd 0.000 zeropoint 0.00 # Output:gnuastro-0.2.33-8a3b/bin/mknoise/Makefile.am0000644000175000017500000000270012765246730015401 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. NOTE: $(top_srcdir)/bootstrapped/lib is only necessary ## for internally compiled utilities and libraries. It must not be included ## during the tests since the bootstrapped libraries are not installed. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Utility and its sources bin_PROGRAMS = astmknoise astmknoise_SOURCES = main.c main.h cite.h ui.c ui.h args.h \ mknoise.c mknoise.h astmknoise_LDADD = $(top_builddir)/bootstrapped/lib/libgnu.la \ -lgnuastro ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astmknoise.conf gnuastro-0.2.33-8a3b/bin/mkcatalog/0000755000175000017500000000000013004464724013713 500000000000000gnuastro-0.2.33-8a3b/bin/mkcatalog/upperlimit.h0000644000175000017500000000242112774004061016172 00000000000000/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __MKCATALOG_UPPERLIMIT_H__ #define __MKCATALOG_UPPERLIMIT_H__ /* Functions: */ float * upperlimit(float *img, float *sky, long *seg, long *mask, size_t s0, size_t s1, size_t upnum, size_t numthreads, int envseed, float sclipmultip, float sclipaccu); #endif gnuastro-0.2.33-8a3b/bin/mkcatalog/upperlimit.c0000644000175000017500000004143713001632540016170 00000000000000/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include "upperlimit.h" /*********************************************************************/ /************ Structures and macros ****************/ /*********************************************************************/ /* These structures and macros are defined in the C file since they are only necessary in the processing here, they do not need to be given to the user through the header, it will just complicate their name-space. */ struct upperlimitparams { size_t s0; /* Number of rows in image. */ size_t s1; /* Number of columns in image. */ int envseed; /* ==1: evironment for rng setup. */ long minlab; /* Minimum label in image. */ long numlabs; /* Number of labels in image. */ float *img; /* The input image. */ size_t *box; /* The box parameters of each label. */ unsigned char **pix; /* The pixels of each label. */ float *std; /* Standard deviation of the sums. */ size_t upnum; /* Number of random samples. */ size_t numthreads; /* Number of threads to use. */ float sclipmultip; /* Multiple of STD for sigma clip. */ float sclipaccu; /* Accuracy to stop sigma clipping. */ }; /* Information for each thread. */ struct tupperlimitparams { size_t id; /* Id of this thread. */ size_t *indexs; /* Indexes for this thread. */ pthread_barrier_t *b; /* Barrier for all threads. */ struct upperlimitparams *p; /* Pointer to main program struct. */ }; /* Columns of labeled region information. Note that the width columns (WIDCOL) are actually the same as the max columns (MAXCOL). The width values are written over the maximum columns because we don't need the maximum values any more. */ #define XMINCOL 0 #define YMINCOL 1 #define XMAXCOL 2 #define YMAXCOL 3 #define XWIDCOL XMAXCOL #define YWIDCOL YMAXCOL /*********************************************************************/ /************ Preparations ****************/ /*********************************************************************/ static void fillseginfo(struct upperlimitparams *p, long *seg) { float *f, *ff; long *l, *ll, maxlab; unsigned char *u, *uu; size_t xw, yw, xmin, ymin; size_t i, j, asize, label, size=p->s0*p->s1; /* Find the minimum and maximum labels: */ maxlab = INT32_MIN; p->minlab = INT32_MAX; ll=(l=seg)+size; do /* We don't want to look at pixels with value zero or blank pixels, so ignore them. */ if( *l!=0 && *l!=GAL_FITS_LONG_BLANK ) { if(*l>maxlab) maxlab=*l; if(*lminlab) p->minlab=*l; } while(++lminlab<0) error(EXIT_FAILURE, 0, "the labeled image must not contain negative " "pixels"); /* Allocate the space to keep the object information. This array will keep the minimum and maximum coordinate for each labeled region. Note that max is in the image, and we want to use the labels as indexs (row numbers), so we must allocate max+1 rows. Note: we are not assuming that the first index is 1. Because many cases can arise where the lowest index can be a large number (for example when the user can be working on a sub-set of objects selected from a large catalog), so we don't want to allocate a huge amount of memory and waste thread resources on them. We have stored the minimum label and will use that in reporting the final output to make a full array. */ p->numlabs = maxlab - p->minlab + 1; errno=0; p->box=malloc(p->numlabs * 4 * sizeof *p->box); if(p->box==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->box", p->numlabs * 4 * sizeof *p->box); /* Initialize the information array*/ for(i=0;inumlabs;++i) { p->box[ i*4 + XMINCOL ] = p->s0; p->box[ i*4 + YMINCOL ] = p->s1; p->box[ i*4 + XMAXCOL ] = p->box[ i*4 + YMAXCOL ] = 0; } /* Fill it in with the minimum and maximum positions. */ for(i=0;is0;++i) for(j=0;js1;++j) if(seg[i*p->s1+j]>0) { label = seg[i*p->s1+j] - p->minlab; if(ibox[ label*4 + XMINCOL ]) p->box[ label*4 + XMINCOL ] = i; if(jbox[ label*4 + YMINCOL ]) p->box[ label*4 + YMINCOL ] = j; if(i>p->box[ label*4 + XMAXCOL ]) p->box[ label*4 + XMAXCOL ] = i; if(j>p->box[ label*4 + YMAXCOL ]) p->box[ label*4 + YMAXCOL ] = j; } /* For a check. Note that in DS9 the coordinates are inverted and start from 1, not zero. { i=0; printf("%zu: (%zu, %zu) --> (%zu, %zu)\n", i+p->minlab, p->box[i*4+YMINCOL]+1, p->box[i*4+XMINCOL]+1, p->box[i*4+YMAXCOL]+1, p->box[i*4+XMAXCOL]+1); } */ /* Allocate the pointers to the object's pixels and allocate space for the area of each detection. In the meantime, Change the xmax and ymax to width in X and width in Y*/ errno=0; p->pix=malloc(p->numlabs * sizeof *p->pix); if(p->pix==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->pix", p->numlabs * sizeof *p->pix); for(i=0; inumlabs; ++i) { /* Replace the max values with the width of each box. */ p->box[i*4+XWIDCOL] = p->box[i*4+XMAXCOL] - p->box[i*4+XMINCOL] + 1; p->box[i*4+YWIDCOL] = p->box[i*4+YMAXCOL] - p->box[i*4+YMINCOL] + 1; /* Allocate space for the pixels of this label. */ errno=0; asize = p->box[i*4+XWIDCOL] * p->box[i*4+YWIDCOL] * sizeof **p->pix; p->pix[i] = malloc(asize); if(p->pix[i]==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->pix[i] (i=%zu)", asize, i); /* Set the array values. Any pixel that is equal to the object's label over the box is given a value of 1.0f, other pixels are given a value of 0.0f. We set the starting pointers for the larger and smaller arrays in this row, then go along the row until it finshes. `j' will take us to the next row after this row finishes. */ xmin = p->box[ i*4+XMINCOL ]; ymin = p->box[ i*4+YMINCOL ]; xw = p->box[ i*4+XWIDCOL ]; yw = p->box[ i*4+YWIDCOL ]; for(j=0; jpix[i] + yw*j ) + yw; l = seg + (xmin+j)*p->s1 + ymin; do *u = (*l++ == i+p->minlab); while(++upix[i], p->box[i*4+XWIDCOL], p->box[i*4+YWIDCOL], 0, NULL, NULL, "myprog"); exit(0); */ /* Allocate an array for the output values, note that this is for the full list of IDs, not just those in the image. */ p->std = malloc( (maxlab+1) * sizeof *p->std ); if(p->std==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->std (upperlimit.c)", (maxlab+1) * sizeof *p->std); ff=(f=p->std)+(maxlab+1); do *f++=NAN; while(fs0*p->s1; /* Allocate the space for the image. */ errno=0; p->img=malloc(size * sizeof *p->img); if(p->img==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->img (upperlimit.c)", size * sizeof *p->img); /* Set the values. */ ff=(f=p->img)+size; do { /* Note that the Sky and mask are optional (can be NULL), so we are checking their existance (not NULL) first. */ if(mask) { *f = *img++ - (( *seg || *mask ) ? NAN : ( sky ? *sky : 0 )); ++mask; } else *f = *img++ - (*seg ? NAN : ( sky ? *sky : 0 )); /* Increment the pointers (when they exist) to the next pixel. */ ++seg; if(sky) ++sky; } while(++fimg, p->s0, p->s1, 0, NULL, NULL, "myprog"); exit(0); */ } /*********************************************************************/ /************ Actual operation on threads ****************/ /*********************************************************************/ static void * upperlimit_on_thread(void *inparam) { /* The first thing to do is to say what the input pointer actually is. */ struct tupperlimitparams *tp = (struct tupperlimitparams *)inparam; struct upperlimitparams *p = tp->p; /* Now you can go onto do defining the function like any other function: first you define the variables and so on... */ double *sum; gsl_rng *rng; unsigned char *u, *uu; float *l, ave, med, *fsum; size_t i, j, c, xw, yw, lab, xmin, ymin; /* Allcate space to keep the total sums */ errno=0; sum=malloc(p->upnum*sizeof *sum); if(sum==NULL) error(EXIT_FAILURE, errno, "%zu bytes for sum (upperlimit.c)", p->upnum*sizeof *sum); /* Allocate the random number generator for this thread. Note that when envseed is non-zero, then we need to use the given environment value. However, we cannot use the same value for all threads because all the positions of all threads will be the same, so we add the thread-id (which is also a known paramter) to the seed. A given number of segments will be distributed between a given number of threads in a reproducible manner, so with this seed value for this thread, we will get reproducible results.*/ rng=gsl_rng_alloc(gsl_rng_default); gsl_rng_set(rng, gsl_rng_default_seed+tp->id); /* Go over the jobs indexed for this thread: */ for(i=0; tp->indexs[i] != GAL_THREADS_NON_THRD_INDEX; ++i) { /* Setup this labels parameters */ c=0; lab=tp->indexs[i]; xw = p->box[ lab*4 + XWIDCOL ]; yw = p->box[ lab*4 + YWIDCOL ]; /* The starting point should be placed between 0 and Image_width - box_width. */ while(cupnum) { /* Get a randomly placed start for this label */ sum[c] = 0.0f; xmin = gsl_rng_uniform_int(rng, p->s0-xw); ymin = gsl_rng_uniform_int(rng, p->s1-yw); /* Go over the pixels and get the sum of the pixel values, this is very similar to the loop in fillseginfo. */ for(j=0; jpix[lab] + yw*j ) + yw; l = p->img + (xmin+j)*p->s1 + ymin; /* We can't simply multiply, since NaN values might be involved over regions that we don't need.*/ do {sum[c] += *u==1.0f ? *l : 0.0f; ++l;} while(++usclipmultip, p->sclipaccu, &ave, &med, &p->std[p->minlab+lab], 0); /* printf("%f\n", p->std[ lab*p->numoutcols + p->nimg ]); exit(0); p->std[ lab*p->numoutcols + p->nimg ] = gsl_stats_sd(sum, 1, c); */ } /* Free the random number generator space. */ free(sum); gsl_rng_free(rng); /* Wait until all other threads finish. When there was only one thread, we explicitly set the pointer to the barrier structure to NULL, so only wait when a barrier is actually defined.*/ if(tp->b) pthread_barrier_wait(tp->b); /* Return the NULL pointer. */ return NULL; } /* This is the thread spinner function. For each image we will divide all the objects between the threads and the */ void upperlimit_manager(struct upperlimitparams *p) { int err; pthread_t t; /* All thread ids saved in this, not used. */ size_t numbarriers; pthread_attr_t attr; pthread_barrier_t b; size_t i, *indexs, thrdcols; struct tupperlimitparams *tp; /* Allocate the array of `param' structures. Note that in most cases, the number of threads will not be a constant like this simple case, it will be a variable passed to the thread-spinner. So we are using dynamic allocation for more general use as a tutorial. */ errno=0; tp = malloc(p->numthreads*sizeof *tp); if( tp==NULL ) error(EXIT_FAILURE, errno, "%zu bytes for tp (upperlimit.c)", p->numthreads*sizeof *tp); /* Distribute the actions into the threads: */ gal_threads_dist_in_threads(p->numlabs, p->numthreads, &indexs, &thrdcols); /* Do the job: when only one thread is necessary, there is no need to spin off one thread, just call the function directly (spinning off threads is expensive). This is for the generic thread spinner function, not this simple function where `p->numthreads' is a constant. */ if(p->numthreads==1) { tp[0].p=p; tp[0].id=0; tp[0].b=NULL; tp[0].indexs=indexs; upperlimit_on_thread(&tp[0]); } else { /* Initialize the attributes. Note that this running thread (that spinns off the nt threads) is also a thread, so the number the barriers should be one more than the number of threads spinned off. */ numbarriers = ( (p->numlabsnumthreads ? p->numlabs : p->numthreads) + 1 ); gal_threads_attr_barrier_init(&attr, &b, numbarriers); /* Spin off the threads: */ for(i=0;inumthreads;++i) if(indexs[i*thrdcols]!=GAL_THREADS_NON_THRD_INDEX) { tp[i].p=p; tp[i].id=i; tp[i].b=&b; tp[i].indexs=&indexs[i*thrdcols]; err=pthread_create(&t, &attr, upperlimit_on_thread, &tp[i]); if(err) { fprintf(stderr, "can't create thread %zu", i); exit(EXIT_FAILURE); } } /* Wait for all threads to finish and free the spaces. */ pthread_barrier_wait(&b); pthread_attr_destroy(&attr); pthread_barrier_destroy(&b); } /* Clean up. */ free(tp); free(indexs); } /*********************************************************************/ /************ External function ****************/ /*********************************************************************/ float * upperlimit(float *img, float *sky, long *seg, long *mask, size_t s0, size_t s1, size_t upnum, size_t numthreads, int envseed, float sclipmultip, float sclipaccu) { size_t i; struct upperlimitparams p; /* Put the input parameters in the structure. */ p.s0=s0; p.s1=s1; p.upnum=upnum; p.envseed=envseed; p.sclipaccu=sclipaccu; p.numthreads=numthreads; p.sclipmultip=sclipmultip; /* Fill the information for each segment. */ fillseginfo(&p, seg); /* Prepare the image. */ prepareimg(&p, img, sky, seg, mask); /* Find the upper limit for all the objects on a thread. */ upperlimit_manager(&p); /* For a check: for(i=1;i Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef COLUMNS_H #define COLUMNS_H /* Units: */ #define CATDESCRIPTLENGTH "%-60s" #define CATUNITRATIO "ratio" #define CATUNITDEGREE "degree" #define CATUNITCOUNTER "counter" #define CATUNITPIXAREA "pixel area" #define CATUNITMAG "scale (log)" #define CATUNITPIXLENGTH "pixel length" #define CATUNITBRIGHTNESS "input data unit" #define CATUNITAVE "("CATUNITBRIGHTNESS")/pixel" /* Fixed names */ #define MKCATX "X" #define MKCATY "Y" #define MKCATRA "RA" #define MKCATDEC "Dec" #define MKCATCLUMP "Clump" #define MKCATMAG "magnitude" #define MKCATBRIGHT "brightness" #define MKCATOBJECT "Full object" #define MKCATWHTC "weighted center" #define MKCATGEOC "geometric center" #define MKCATCINO "Clumps in object" #define MKRIVERSSUR "Rivers surrounding clump, average" void idcol(struct mkcatalogparams *p); void hostobj(struct mkcatalogparams *p, int o1c0); void numclumps(struct mkcatalogparams *p); void area(struct mkcatalogparams *p, int cinobj, int isriver); void position(struct mkcatalogparams *p, size_t col, char *target, char *type, char *axis); void secondordermoment(struct mkcatalogparams *p, size_t ocol, char *target); void brightnessmag(struct mkcatalogparams *p, size_t col, char *target, char *scale); void upperlimitcol(struct mkcatalogparams *p); void skystd(struct mkcatalogparams *p, size_t col); void sncol(struct mkcatalogparams *p, int sn0_magerr1, char *target); #endif gnuastro-0.2.33-8a3b/bin/mkcatalog/columns.c0000644000175000017500000010144513001632537015460 00000000000000/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. ABOUT THIS FILE: The information tables are fully explained in the comments of main.h. After the raw information is read in the first and second pass, the job of the functions here is to process the raw columns that are needed into useful knowledge and print them. for example those functions will only record the weighted sum of pixel positions and the total weight, here the weighted sum is divided by the total weight to yeild an average. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include "main.h" #include "columns.h" #include "mkcatalog.h" #include "upperlimit.h" /******************************************************************/ /******* Information table modifications *************/ /******************************************************************/ /* Correct the average Sky and Sky standard deviation value for objects and clumps. Note that during the passes, these were just sums of pixel values, they need to be divided by the area of the object/clump, which is done here. */ void setskystd(struct mkcatalogparams *p, size_t col) { size_t ac; double *row = p->info + p->icols; double *end = row + (p->icols * p->num); /* Only do the correction if this column is not already flagged. */ if(p->info[col]==0.0f) { /* Set the area column: */ ac = p->obj0clump1 ? CALLAREA : OALLAREA; /* Go over every row and do the correction. */ do { row[col] = ( row[ac]>0.0f ? row[col]/row[ac] : NAN ); row+=p->icols; } while(rowinfo[col]=1.0f; } } /* Correct the average river value, after the passes, it is just the sum. */ void setaveriver(struct mkcatalogparams *p) { double *row = p->info + p->icols; double *end = row + (p->icols * p->num); /* Only do the correction if this column is not already flagged. */ if(p->info[CRivAve]==0.0f) { /* Make sure the Sky values are corrected */ setskystd(p, CSKY); /* Go over every row and do the correction. Note that in cases where the grown clumps are used instead of the clumps, we are not going to have any rivers (row[CRivArea]==0.0f). In such situations, set the per-pixel average river value to the Sky value under the clump. The reason is that for the clumps, Sky subtraction was not done on the Clump brightness, so this value will be used, and if there was no river, then we need something to replace it. */ do { row[CRivAve] = ( row[CRivArea]>0.0f ? row[CRivAve]/row[CRivArea] : row[CSKY] ); row+=p->icols; } while(rowinfo[CRivAve]=1.0f; } } /* The clump brightness values are not Sky subtracted since the river values (which are also not Sky subtracted) should be subtracted from them. Here that job is done. */ void setclumpbrightness(struct mkcatalogparams *p) { double *row = p->info + p->icols; double *end = row + (p->icols * p->num); /* Only do the correction if this column is not already flagged. */ if(p->info[CBrightness]==0.0f) { /* Make sure the average river value is calculated */ setaveriver(p); /* On a clump, we have to subtract the average river flux multiplied by the the area of the clump. The value in the CBrightness column is simply the sum of pixels. Note that here we are multiplying by the area of the clump (CALLAREA) irrespective of threshold, while in setaveriver(), we divided by the area of the river (CRivArea). */ do { row[CBrightness] -= row[CRivAve]*row[CAREA]; row+=p->icols; } while(rowinfo[CBrightness]=1.0f; } } /* Find the geometric center of the profile (average position, ignoring any flux of the pixels). */ void geoxy(struct mkcatalogparams *p, size_t col) { size_t ac=-1; double *row = p->info + p->icols; double *end = row + (p->icols * p->num); /* Only if this column is not flagged as already done (==1.0f). */ if(p->info[col]==0.0f) { /* First, set the columns to use for the conversion. */ if(p->obj0clump1) ac=CAREA; else { if (col==OGeoX || col==OGeoY) ac=OAREA; else if (col==OGeoCX || col==OGeoCY) ac=OAREAC; else error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we " "can fix this. The given column in the --OBJECTS-- " "information table was not recognized for calculating the " "geometric X and/or Y", PACKAGE_BUGREPORT); } /* Go over all the rows and correct this column. */ do { /* Set the value for this row. Note that unlike the calculations here that start counting with zero, the FITS standard starts counting from 1, so add a one after dividing by the area. If the area is zero, then set NaN. */ row[col] = row[ac]>0.0f ? row[col] / row[ac] : NAN; /* Go onto the next row: */ row+=p->icols; } while(rowinfo[col]=1.0f; } } /* A low-level function used to find the flux weighted center, since it is needed by multiple columns. The geometric center for this axis colum (geocol) and area column (areacol) are needed for backup (when there might not be any positive flux pixel/data values to use for weight). */ void flxwhtimg(struct mkcatalogparams *p, size_t col) { size_t wc=-1, gc=-1; double *row = p->info + p->icols; double *end = row + (p->icols * p->num);; /* Only if this column is not flagged as already done (==1.0f). */ if(p->info[col]==0.0f) { /* First, set the columns to use for the conversion. */ if(p->obj0clump1) { wc=CPosBright; if (col==CFlxWhtX) gc=CGeoX; else if(col==CFlxWhtY) gc=CGeoY; else error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we " "can fix this. The given column in the --CLUMPS-- " "information table was not recognized for calculating the " "final flux weighted X and/or Y", PACKAGE_BUGREPORT); } else { if (col==OFlxWhtX || col==OFlxWhtY) { wc=OPosBright; gc = col==OFlxWhtX ? OGeoX : OGeoY; } else if (col==OFlxWhtCX || col==OFlxWhtCY) { wc=OPosBrightC; gc = col==OFlxWhtCX ? OGeoCX : OGeoCY; } else error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we " "can fix this. The given column in the --OBJECTS-- " "information table was not recognized for calculating the " "final flux weighted X and/or Y", PACKAGE_BUGREPORT); } /* The geometric positions act as a backup for the flux weighted centers, so make sure the appropriate geometric center is defined. */ geoxy(p, gc); /* For a check, uncomment these two lines: printf("\n\nInfocol: %zu (%s, %zu)\n", col, p->info==p->oinfo?"Objects":"Clumps", p->num); Then add these two lines before and after row[col] in the loop*/ /*printf("%zu: %f --> ", (row-p->info)/p->icols, row[col]);*/ /*printf("%f\n", row[col]);*/ /* Go over all the rows and correct this column. */ do { /* Set the value for this row. When a positive weight is present, we are adding with one (1) because of the FITS standard. */ row[col] = row[wc]>0.0f ? (row[col]/row[wc]) : row[gc]; /* Go onto the next row: */ row+=p->icols; } while(rowinfo[col]=1.0f; } } /* To correct the second moment, we need three variables: the first moment in first axis, first moment in second axis and the total weight. The first two are the same when the second moment is a power of one axis. The weight is either the total positive flux used for the weights, or is the area. */ void setsecondmoment(struct mkcatalogparams *p, size_t col) { double *row = p->info + p->icols; double *end = row + (p->icols * p->num); size_t fc=-1, sc=-1, wc=-1, sfc=-1, ssc=-1; /* Only if this column is not flagged as already done (==1.0f). */ if(p->info[col]==0.0f) { /* First, set the columns to use for the conversion. Note that since we also need to correct the column, we have merged the setting of fc and sc and the calling of the flxwhtimg function into one call. */ if(p->obj0clump1) switch(col) { /* Clump brightness weighted */ case CFlxWhtXX: wc=CPosBright; fc=sc=CFlxWhtX; flxwhtimg(p, fc); sfc=ssc=CPOSSHIFTX; break; case CFlxWhtYY: wc=CPosBright; fc=sc=CFlxWhtY; flxwhtimg(p, fc); sfc=ssc=CPOSSHIFTY; break; case CFlxWhtXY: wc=CPosBright; flxwhtimg(p, fc=CFlxWhtX); flxwhtimg(p, sc=CFlxWhtY); sfc=CPOSSHIFTX; ssc=CPOSSHIFTY; break; /* Clump geometric: */ case CGeoXX: wc=CAREA; fc=sc=CGeoX; geoxy(p, fc); sfc=ssc=CPOSSHIFTX; break; case CGeoYY: wc=CAREA; fc=sc=CGeoY; geoxy(p, fc); sfc=ssc=CPOSSHIFTY; break; case CGeoXY: wc=CAREA; geoxy(p, fc=CGeoX); geoxy(p, sc=CGeoY); sfc=CPOSSHIFTX; ssc=CPOSSHIFTY; break; default: error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we " "can fix this. The given column in setsecondmoment's " "--CLUMP-- information table (%zu) was not recognized for " "correcting the second moment", PACKAGE_BUGREPORT, col); } else switch(col) { /* All object brightness weighted: */ case OFlxWhtXX: wc=OPosBright; fc=sc=OFlxWhtX; flxwhtimg(p, fc); sfc=ssc=OPOSSHIFTX; break; case OFlxWhtYY: wc=OPosBright; fc=sc=OFlxWhtY; flxwhtimg(p, fc); sfc=ssc=OPOSSHIFTY; break; case OFlxWhtXY: wc=OPosBright; flxwhtimg(p, fc=OFlxWhtX); flxwhtimg(p, sc=OFlxWhtY); sfc=OPOSSHIFTX; ssc=OPOSSHIFTY; break; /* All object geometric: */ case OGeoXX: wc=OAREA; fc=sc=OGeoX; geoxy(p, fc); sfc=ssc=OPOSSHIFTX; break; case OGeoYY: wc=OAREA; fc=sc=OGeoY; geoxy(p, fc); sfc=ssc=OPOSSHIFTY; break; case OGeoXY: wc=OAREA; geoxy(p, fc=OGeoX); geoxy(p, sc=OGeoY); sfc=OPOSSHIFTX; ssc=OPOSSHIFTY; break; /* Clumps in object brightness weighted: */ case OFlxWhtCXX: wc=OPosBrightC; fc=sc=OFlxWhtCX; flxwhtimg(p, fc); sfc=ssc=OPOSSHIFTX; break; case OFlxWhtCYY: wc=OPosBrightC; fc=sc=OFlxWhtCY; flxwhtimg(p, fc); sfc=ssc=OPOSSHIFTY; break; case OFlxWhtCXY: wc=OPosBrightC; flxwhtimg(p, fc=OFlxWhtCX); flxwhtimg(p, sc=OFlxWhtCY); sfc=OPOSSHIFTX; ssc=OPOSSHIFTY; break; /* Clumps in object geometric: */ case OGeoCXX: wc=OAREAC; fc=sc=OGeoCX; geoxy(p, fc); sfc=ssc=OPOSSHIFTX; break; case OGeoCYY: wc=OAREAC; fc=sc=OGeoCY; geoxy(p, fc); sfc=ssc=OPOSSHIFTY; break; case OGeoCXY: wc=OAREAC; geoxy(p, fc=OGeoCX); geoxy(p, sc=OGeoCY); sfc=OPOSSHIFTX; ssc=OPOSSHIFTY; break; default: error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we " "can fix this. The given column in setsecondmoment's " "--OBJECT-- information table (%zu) was not recognized for " "correcting the second moment", PACKAGE_BUGREPORT, col); } /* Go over all the rows and correct this column. */ do { /* Set the value for this row, including the shift in calculating the second order moments. */ row[col] = ( row[col]/row[wc] - (row[fc]-row[sfc]) * (row[sc]-row[ssc]) ); /* Go onto the next row: */ row+=p->icols; } while(rowinfo[col]=1.0f; } } /* Fill in the RA and Dec columns, note that we will need the X and Y colums first for this. */ void preparewcs(struct mkcatalogparams *p, size_t col) { /* Initialize all the columns to -1 (largest possible number in the C's unsigned char, so if there is any bugs, we get a good error. */ int wht0geo1=-1; size_t xc=-1, yc=-1, rc=-1, dc=-1; /* RA and Dec are usually needed together and must also be calculated together, but here, we are giving the user complete freedom in setting the columns in which ever order they want. So after calculating the RA and Dec once for either of the two, there is no more need to do the calculation again. */ if(p->info[col]==0.0f) { /* First, set the columns to use for the conversion. */ if(p->obj0clump1) { /* Clump, flux weighted: */ if(col==CFlxWhtRA || col==CFlxWhtDec) { xc=CFlxWhtX; yc=CFlxWhtY; rc=CFlxWhtRA; dc=CFlxWhtDec; wht0geo1=0; } /* Clump, geometric: */ else if(col==CGeoRA || col==CGeoDec) { xc=CGeoX; yc=CGeoY; rc=CGeoRA; dc=CGeoDec; wht0geo1=1; } else error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we " "can fix this. The given column in the --CLUMPS-- " "information table was not recognized for calculating the " "RA and Dec", PACKAGE_BUGREPORT); } else { /* All clumps in object, flux weighted: */ if(col==OFlxWhtCRA || col==OFlxWhtCDec) { xc=OFlxWhtCX; yc=OFlxWhtCY; rc=OFlxWhtCRA; dc=OFlxWhtCDec; wht0geo1=0; } /* All clumps in object, geometric: */ else if(col==OGeoCRA || col==OGeoCDec) { xc=OGeoCX; yc=OGeoCY; rc=OGeoCRA; dc=OGeoCDec; wht0geo1=1; } /* All object, flux weighted */ else if(col==OFlxWhtRA || col==OFlxWhtDec) { xc=OFlxWhtX; yc=OFlxWhtY; rc=OFlxWhtRA; dc=OFlxWhtDec; wht0geo1=0; } /* All object, geometric */ else if(col==OGeoRA || col==OGeoDec) { xc=OGeoX; yc=OGeoY; rc=OGeoRA; dc=OGeoDec; wht0geo1=1; } else error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we " "can fix this. The given column in the --OBJECT-- " "information table was not recognized for calculating the " "RA and Dec", PACKAGE_BUGREPORT); } /* Finalize the relevant X and Y positions first (which are needed for the WCS conversion). Note that if they are ready to use (their flag is 1.0f), these functions will not do anything. But if the user hasn't already asked for X and Y, then these columns will be corrected here.*/ switch(wht0geo1) { case 0: flxwhtimg(p, xc); flxwhtimg(p, yc); break; case 1: geoxy(p, xc); geoxy(p, yc); break; default: error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we " "can fix this. The value of the wht0geo1 variable (%d) is " "not recognized", PACKAGE_BUGREPORT, wht0geo1); } /* Do the conversion. Note that the p->icols is added because the first row is not used by any object or colump (since their indexes begin from 1).*/ gal_wcs_xy_array_to_radec(p->wcs, p->info+p->icols+xc, p->info+p->icols+rc, p->num, p->icols); /* Set the flag of the converted columns to 1.0f, so the calculations are not repeated if any of the columns is needed again. Note that it is irrelevant which one of the RA or Dec were calculated, so we are not using `col' here. */ p->info[rc]=p->info[dc]=1.0f; } } /******************************************************************/ /*************** Add columns for printing *******************/ /******************************************************************/ void idcol(struct mkcatalogparams *p) { size_t i; p->unitp=CATUNITCOUNTER; sprintf(p->description, "%zu: Overall %s ID", p->curcol, p->name); for(i=0;inum;++i) p->cat[ i * p->numcols + p->curcol ] = i+1; p->intcols[p->intcounter++]=p->curcol; } /* Store IDs related to the host object: o1c0==1 --> hostobjid: The ID of object hosting this clump o1c0==0 --> idinhostobj: The ID of clump in object */ void hostobj(struct mkcatalogparams *p, int o1c0) { char *des; double counter; size_t i, j, n, row=0; p->unitp=CATUNITCOUNTER; des = ( o1c0 ? "ID of object hosting this clump" : "ID of clump in host object" ); sprintf(p->description, "%zu: %s.", p->curcol, des); for(i=1;i<=p->numobjects;++i) if( (n=p->oinfo[i*OCOLUMNS+ONCLUMPS]) > 0.0f) { counter=1.0f; for(j=row;jcat[ j * p->numcols + p->curcol] = o1c0 ? i : counter++; row+=n; } p->intcols[p->intcounter++]=p->curcol; } void numclumps(struct mkcatalogparams *p) { size_t i; p->unitp=CATUNITCOUNTER; sprintf(p->description, "%zu: Number of clumps in this object.", p->curcol); for(i=0;inumobjects;++i) p->cat[i * p->numcols + p->curcol ] = p->oinfo[(i+1)*OCOLUMNS+ONCLUMPS]; p->intcols[p->intcounter++]=p->curcol; } void area(struct mkcatalogparams *p, int cinobj, int isriver) { char *type; size_t i, col; /* Set the proper column to use */ if(p->obj0clump1) { if(isriver) { type="Number of river pixels around this clump"; col=CRivArea; } else { type = isnan(p->threshold) ? "Area of this clump" : "Area of this clump above threshold"; col = CAREA; } } else { if(cinobj) /* It is the positions of clumps in object. */ { type="Clumps in object area"; col = OAREAC; } else /* It is the position of the object itsself.*/ { type="Full object area"; col = OAREA; } } /* Set the unit and print the header. */ p->unitp = isriver ? CATUNITCOUNTER : CATUNITPIXAREA; sprintf(p->description, "%zu: %s.", p->curcol, type); /* Fill in the output array. */ for(i=0;inum;++i) p->cat[i * p->numcols + p->curcol ] = p->info[(i+1)*p->icols+col]; /* Set the precision for printing. */ p->intcols[p->intcounter++]=p->curcol; } void position(struct mkcatalogparams *p, size_t col, char *target, char *type, char *axis) { size_t i; int wcsax = ( !strcmp(axis, MKCATRA) || !strcmp(axis, MKCATDEC) ) ? 1 : 0; /* Set the header information. */ sprintf(p->description, "%zu: %s %s (%s).", p->curcol, target, type, axis); /* Prepare the respective column, set the units and also the printing accuracy if we are in RA/Dec mode (wcsax==1). */ if(wcsax) { /* Run the respective function to prepare the information table, then set the units and print accuracy. */ preparewcs(p, col); p->unitp = CATUNITDEGREE; p->accucols[p->accucounter++]=p->curcol; } else { /* Run the respective function to prepare the information table. */ if(!strcmp(type, MKCATGEOC)) geoxy(p, col); else if(!strcmp(type, MKCATWHTC)) flxwhtimg(p, col); else error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we can " "solve this problem. The value to `type' (%s) is not " "recognized in position (image mode)", PACKAGE_BUGREPORT, type); /* Set the units. */ p->unitp = CATUNITPIXLENGTH; } /* Write respective column of the information table into the output. */ for(i=0;inum;++i) p->cat[i * p->numcols + p->curcol ] = p->info[(i+1)*p->icols+col]; } /* Note that here, the output column is used, not the input one. */ void secondordermoment(struct mkcatalogparams *p, size_t ocol, char *target) { double a, *row; char *name=NULL, *type=NULL; size_t i, xxc=-1, yyc=-1, xyc=-1; /* Set the necessary columns, and the type of output: */ switch(ocol) { /* The brightness weighted second moments. */ case CATSEMIMAJOR: case CATSEMIMINOR: case CATPOSITIONANGLE: type="weighted"; if(p->obj0clump1) {xxc=CFlxWhtXX; yyc=CFlxWhtYY; xyc=CFlxWhtXY;} else {xxc=OFlxWhtXX; yyc=OFlxWhtYY; xyc=OFlxWhtXY;} break; /* The geometric second moments. */ case CATGEOSEMIMAJOR: case CATGEOSEMIMINOR: case CATGEOPOSITIONANGLE: type="geometric"; if(p->obj0clump1) {xxc=CGeoXX; yyc=CGeoYY; xyc=CGeoXY;} else {xxc=OGeoXX; yyc=OGeoYY; xyc=OGeoXY;} break; /* Output column not recognized */ default: error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we can " "solve this problem. The value to `ocol' (%zu) is not " "recognized in secondordermoment (first)", PACKAGE_BUGREPORT, ocol); } /* Prepare the columns which will be needed in the next step. */ setsecondmoment(p, xxc); setsecondmoment(p, yyc); setsecondmoment(p, xyc); /* Set output name and do the calculation, the calculations are taken from the SExtractor manual. */ switch(ocol) { case CATSEMIMAJOR: case CATGEOSEMIMAJOR: name="semi major axis"; p->unitp = CATUNITPIXLENGTH; for(i=0;inum;++i) { row = p->info + (i+1)*p->icols; a=(row[xxc]-row[yyc])*(row[xxc]-row[yyc])/4; p->cat[i * p->numcols + p->curcol ] = sqrt( (row[xxc]+row[yyc])/2 + sqrt( a + row[xyc]*row[xyc]) ); } break; case CATSEMIMINOR: case CATGEOSEMIMINOR: name="semi minor axis"; p->unitp = CATUNITPIXLENGTH; for(i=0;inum;++i) { row = p->info + (i+1)*p->icols; a=(row[xxc]-row[yyc])*(row[xxc]-row[yyc])/4; p->cat[i * p->numcols + p->curcol ] = sqrt( (row[xxc]+row[yyc])/2 - sqrt( a + row[xyc]*row[xyc]) ); } break; case CATPOSITIONANGLE: case CATGEOPOSITIONANGLE: name="position angle"; p->unitp = CATUNITDEGREE; for(i=0;inum;++i) { row = p->info + (i+1)*p->icols; p->cat[i * p->numcols + p->curcol ] = 0.5*atan2(2*row[xyc], row[xxc]-row[yyc]) * 180/M_PI; } break; default: error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we can " "solve this problem. The value to `ocol' (%zu) is not " "recognized in secondordermoment (second)", PACKAGE_BUGREPORT, ocol); } /* Set the header value */ sprintf(p->description, "%zu: %s %s %s.", p->curcol, target, type, name); } void brightnessmag(struct mkcatalogparams *p, size_t col, char *target, char *scale) { size_t i; char *add; double bright, *value; /* Prepare other necessary columns */ if( !strcmp(MKRIVERSSUR, target) ) setaveriver(p); if( !strcmp(MKCATCLUMP, target) && col!=CNoRiverBrightness ) setclumpbrightness(p); /* Fill the output columns: */ for(i=0;inum;++i) { /* Set the basic values: */ bright = p->info[ (i+1) * p->icols + col ]; value = &p->cat[i * p->numcols + p->curcol ]; /* Do the job: */ if(!strcmp(MKCATMAG, scale)) *value = bright<=0.0f ? NAN : -2.5f*log10(bright)+p->zeropoint; else if(!strcmp(MKCATBRIGHT, scale)) *value = bright; else error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we can " "fix this issue. For some reason, the value to `scale' in" "brightnessfluxmag (columns.c) is `%s', which is not " "recognized", PACKAGE_BUGREPORT, scale); } /* Make final preparations for output. When dealing with the average river value, set the accuracy to high, also set the units to average values (per pixel). */ if(!strcmp(MKRIVERSSUR, target)) { p->unitp = CATUNITAVE; p->accucols[p->accucounter++]=p->curcol; } else p->unitp = strcmp(MKCATMAG, scale) ? CATUNITBRIGHTNESS : CATUNITMAG; /* Set the header information: */ add = (col==CNoRiverBrightness) ? " sky (not river) subtracted " : " "; sprintf(p->description, "%zu: %s%s%s.", p->curcol, target, add, scale); } void upperlimitcol(struct mkcatalogparams *p) { size_t i; float *std; double *ptr; /* For the comments: */ p->unitp = CATUNITMAG; sprintf(p->description, "%zu: Upper limit magnitude for this %s.", p->curcol, p->name); /* Correct the raw values (divide them by area) if not already done. */ std=upperlimit(p->img, p->sky, p->objects, p->upmask, p->s0, p->s1, p->upnum, p->cp.numthreads, p->envseed, p->upsclipmultip, p->upsclipaccu); /* Write the standard deviations values in the final catalog as magnitudes. */ for(i=0;inum;++i) { /* `ptr' is defined for a short/readable line. */ ptr = &p->cat[i * p->numcols + p->curcol ]; *ptr = -2.5f * log10( p->upnsigma*std[i+1] ) + p->zeropoint; } free(std); } void skystd(struct mkcatalogparams *p, size_t col) { size_t i; /* For the comments: */ p->unitp = CATUNITAVE; sprintf(p->description, "%zu: Average %s under this %s.", p->curcol, ( (col==OSKY || col==CSKY) ? "sky" : "sky standard deviation" ), p->name); /* Correct the raw values (divide them by area) if not already done. */ setskystd(p, col); /* Fill the sky value, note that in the information array, we have only calculated the sum. So here, we need to divide by the area to find the average. */ for(i=0;inum;++i) p->cat[i * p->numcols + p->curcol ] = p->info[(i+1)*p->icols+col]; /* This column should be accurate: */ p->accucols[p->accucounter++]=p->curcol; } void sncol(struct mkcatalogparams *p, int sn0_magerr1, char *target) { size_t i; double sn, I, O, Ni, errpt, *row; size_t stdcol = p->obj0clump1 ? CSTD : OSTD; size_t areacol = p->obj0clump1 ? CAREA : OAREA; size_t brightnesscol = p->obj0clump1 ? CBrightness : OBrightness; /* Do the corrections: 1. If we are dealing with clumps, make sure the clump brightness is corrected first. 2. Make sure the STD values are corrected in any case. */ setskystd(p, stdcol); if(p->obj0clump1) setclumpbrightness(p); /* For the comments: */ p->unitp = sn0_magerr1 ? CATUNITMAG : CATUNITRATIO; if(sn0_magerr1) sprintf(p->description, "%zu: %s Magnitude error.", p->curcol, target); else sprintf(p->description, "%zu: %s signal to noise ratio.", p->curcol, target); /* Calculate the signal to noise ratio. Recall that for the objects, the sky value was subtracted from oinfo, but for the clumps, it was not subtracted. */ for(i=0;inum;++i) { /* Some convenience variables to make things readable. */ row = p->info + ((i+1)*p->icols); /* Pointer to this row. */ Ni = row[ areacol ]; /* Number-in */ I = row[ brightnesscol ]/Ni; /* Inner brightness (average) */ errpt = row[ stdcol ]*row[ stdcol ]; /* error-to-power-two */ /* If we are on a clump and there are actually rivers (NOTE: it is possible that there are no rivers, see the NoiseChisel dropout paper). In short, they are actually objects with no more than one clump. So, NoiseChisel parameters were set such that the objects also show up in the clumps labels. */ if(p->obj0clump1 && row[ CRivArea ]>0.0f) { /* Another convenience variable. */ O=row[ CRivAve ]; /* Outer brightness (average)*/ /* Modify the error based on the conditions. Note that the inner flux has already been subtracted from the average outer flux multiplied by the clump area in setclumpbrightness and was divided by the clump area above. It is also in per pixel units. row[CRivAve] is also in per pixel units. So simply by adding the two, we get the per pixel flux within the clump before removing the average river value. If the image was already Sky subtracted, then the Sky error^2 (=err) must be multiplied by 2 (we have implicitly used it in both estimating the inner and outer fluxes). Otherwise, it is multiplied by 0.0f, since we don't care because we are not using the Sky value here. */ errpt = ( ( I+O > 0.0f ? I+O : 0.0f ) + ( O > 0.0f ? O : 0.0f ) + errpt * (p->skysubtracted ? 2.0f : 0.0f) ); } else { /* When the flux is negative (can easily happen in matched photometry), then ignore the error in flux (the S/N is meaningless anyway) and just keep the Sky error. When the image was already Sky subtracted, we need two errpt terms, because the error in the previous Sky subtraction must also be included. */ errpt = ( ( I>0 ? I : 0 ) + errpt * (p->skysubtracted ? 1.0f : 2.0f) ); } /* Fill in the output column. Note that magnitude error is directly derivable from the S/N: To derive the error in measuring the magnitude from the S/N, let's take `F' as the flux, `Z' is the zeropoint, `M' is the magnitude, `S' is the S/N, and `D' to stand for capital delta (or error in a value) then from `M = -2.5*log10(F) + Z' we get the following equation after calculating the derivative with respect to F. `dM/df = -2.5 * ( 1 / ( F * ln(10) ) )' From the Tailor series, `DM' can be written as: `DM = dM/dF * DF' So `DM = |-2.5/ln(10)| * DF/F' But `DF/F' is just the inverse of the Signal to noise ratio, or `1/S'. So `DM = 2.5 / ( S * ln(10) )' */ sn = sqrt(Ni/p->cpscorr)*I / sqrt( errpt ); p->cat[i * p->numcols + p->curcol ] = ( sn0_magerr1 ? ( 2.5 / (sn*log(10)) ) : sn ); } } gnuastro-0.2.33-8a3b/bin/mkcatalog/mkcatalog.h0000644000175000017500000000240012616616510015742 00000000000000/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MKCATALOG_H #define MKCATALOG_H #define WNGBSIZE 20 /* wngb: indexs of river neighbors. */ #define COMMENTSIZE 10000 #define COLINFOINT 1 #define COLINFOFLOAT 2 #define COLINFOACCU 3 void mkcatalog(struct mkcatalogparams *p); #endif gnuastro-0.2.33-8a3b/bin/mkcatalog/mkcatalog.c0000644000175000017500000006635013001632537015747 00000000000000/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include "main.h" #include "columns.h" #include "mkcatalog.h" /*********************************************************************/ /***************** Fill information tables *******************/ /*********************************************************************/ /* Macro to see if the label is indexable (belongs to an object or not). See the explanation in bin/noisechisel/label.h. */ #if GAL_FITS_LONG_BLANK<0 #define ISINDEXABLEOBJLABEL (objects[i]>0) #define ISINDEXABLECLPLABEL (clumps[i]>0) #else #define ISINDEXABLEOBJLABEL (objects[i] && objects[i]!=GAL_FITS_LONG_BLANK) #define ISINDEXABLECLPLABEL (clumps[i] && clumps[i]!=GAL_FITS_LONG_BLANK) #endif /* In the first pass, the most basic properties (mainly about the objects) are found. The primary reason is that we still don't know how many objects there are in order to be able to put the clump information in the proper place. This could maybe be fixed with a linked list in one pass, but that would drastically bring down the speed. */ void firstpass(struct mkcatalogparams *p) { float imgss; size_t i, is1=p->s1; double x, y, sx, sy, *thisobj; long *objects=p->objects, *clumps=p->clumps; /* Go over the pixels and fill the information array. */ for(i=0;is0*p->s1;++i) if(ISINDEXABLEOBJLABEL) { /* thisobj is a pointer to the start of the row in the object information array (oinfo). It is mainly used to keep things short, simple, less bugy and most importantly: elegant. */ imgss = p->img[i] - p->sky[i]; thisobj = p->oinfo + objects[i]*OCOLUMNS; /* Set the shifts to avoid round-off errors in large numbers for the non-linear calculations. We are using the first pixel of each object as the shift parameter to keep the mean reasonably near to the standard deviation. Otherwise, when the object is far out in the image (large x and y positions), then roundoff errors are going to decrease the accuracy of the second order calculations. When the object and clumps columns were allocated, the shift columns were set to NaN so we know when to set them for each object/clump. For later parallelization, a mutex can be set up within the `if' statement below and another check can be done within the mutex, this way, only if separate threads get to the start of an object in their respective mesh, for an object that doesn't have a shift already assigned to it, at the same time (highly unlikely) will the process be slightly slowed down. Otherwise, there will be no speed penalty. */ if(isnan(thisobj[ OPOSSHIFTX ])) { thisobj[ OPOSSHIFTX ] = i%is1+1; thisobj[ OPOSSHIFTY ] = i/is1+1; } /* Set the positional variables: */ x = i%is1+1; y = i/is1+1; sx = x - thisobj[ OPOSSHIFTX ]; sy = y - thisobj[ OPOSSHIFTY ]; /* Properties that are independent of threshod: */ ++thisobj[OALLAREA]; thisobj[ OSKY ] += p->sky[i]; thisobj[ OSTD ] += p->std[i]; /* Only if the pixel is above the desired threshold. REASON: The reason this condition is given like this that we don't want to do multiple checks. The basic idea is this: when the user doesn't want any thresholds applied, then p->threshold=NAN and any conditional that involves a NaN will fail, so its logical negation will be positive and the calculations below will be done. However, if the user does specify a threhold and the pixel is above the threshold, then (imgssthreshold*p->std[i]) will be false and its logigal negation will be positive, so the pixel will be included.*/ if(!(imgssthreshold*p->std[i])) { ++thisobj[OAREA]; thisobj[ OGeoX ] += x; thisobj[ OGeoY ] += y; thisobj[ OGeoXX ] += sx * sx; thisobj[ OGeoYY ] += sy * sy; thisobj[ OGeoXY ] += sx * sy; thisobj[ OBrightness ] += imgss; if(imgss>0) { thisobj[ OPosBright ] += imgss; thisobj[ OFlxWhtX ] += imgss * x; thisobj[ OFlxWhtY ] += imgss * y; thisobj[ OFlxWhtXX ] += imgss * sx * sx; thisobj[ OFlxWhtYY ] += imgss * sy * sy; thisobj[ OFlxWhtXY ] += imgss * sx * sy; } } if(clumps && clumps[i]>0) { /* The largest clump ID over each object is the number of clumps that object has. */ thisobj[ ONCLUMPS ] = ( clumps[i] > thisobj[ONCLUMPS] ? clumps[i] : thisobj[ONCLUMPS] ); /* Only if the pixel is above the desired threshold, see explanation under similar condition above. */ if(!(imgssthreshold*p->std[i])) { /* Save the information. */ ++thisobj [ OAREAC ]; thisobj[ OBrightnessC ] += imgss; thisobj[ OGeoCX ] += x; thisobj[ OGeoCY ] += y; thisobj[ OGeoCXX ] += sx * sx; thisobj[ OGeoCYY ] += sy * sy; thisobj[ OGeoCXY ] += sx * sy; if(imgss>0) { thisobj[ OPosBrightC ] += imgss; thisobj[ OFlxWhtCX ] += imgss * x; thisobj[ OFlxWhtCY ] += imgss * y; thisobj[ OFlxWhtCXX ] += imgss * sx * sx; thisobj[ OFlxWhtCYY ] += imgss * sy * sy; thisobj[ OFlxWhtCXY ] += imgss * sx * sy; } } } } } /* In the second pass, we have the number of clumps so we can find the total values for the clumps. */ void clumppass(struct mkcatalogparams *p) { float imgss; double x, y, sx, sy; long wngb[2*WNGBSIZE]; size_t ii, *n, *nf, numngb, ngb[8]; double *thisclump, *cinfo=p->cinfo; long *objects=p->objects, *clumps=p->clumps; float *img=p->img, *sky=p->sky, *std=p->std; size_t i, j, *ind, *ofcrow, row=0, is0=p->s0, is1=p->s1; /* The job of ofcrow (object-first-clump-row) is to give the row number of the first clump within an object in the clumps information table. This value can be added with the clumpid in order to give the row number in the clumps information table. */ errno=0; ofcrow=malloc((p->numobjects+1)*sizeof *ofcrow); if(ofcrow==NULL) error(EXIT_FAILURE, errno, "%zu bytes for ofcrow in seconpass " "(mkcatalog.c)", (p->numobjects+1)*sizeof *ofcrow); /* Fill ofcrow using the known number of clumps in each object. Note that while ofcrow counts from zero, the clump[i] values (which are added with this later) are added with one. So the clump information will start from the second row (with index 1) of the clumps array, not the first (with index 0). */ for(i=1;i<=p->numobjects;++i) if(p->oinfo[i*OCOLUMNS+ONCLUMPS]>0.0f) { ofcrow[i]=row; row+=p->oinfo[i*OCOLUMNS+ONCLUMPS]; } /* Go over all the pixels in the image and fill in the clump information: */ for(i=0;is0*p->s1;++i) { /* We are on a clump, save its properties. */ if(ISINDEXABLECLPLABEL) { /* This pointer really simplifies things below! */ thisclump = ( cinfo + ( ofcrow[objects[i]] + clumps[i] ) * CCOLUMNS ); /* Set the shifts for this object if not already set, see the explanations in the firstpass function. */ if(isnan(thisclump[ CPOSSHIFTX ])) { thisclump[ CPOSSHIFTX ] = i%is1+1; thisclump[ CPOSSHIFTY ] = i/is1+1; } /* Set the positional variables: */ x = i%is1+1; y = i/is1+1; sx = x - thisclump[ CPOSSHIFTX ]; sy = y - thisclump[ CPOSSHIFTY ]; /* Calculations that are independent of the threshold. The CALLAREA is the full area of the clump irrespective of the threshold, this is needed to correctly implement the average river flux (which is defined by the. */ ++thisclump[ CALLAREA ]; thisclump[ CSKY ] += sky[i]; thisclump[ CSTD ] += std[i]; /* Only if the pixel is above the desired threshold, see explanation under similar condition above. */ if(!(img[i]-sky[i]threshold*p->std[i])) { /* Sky subtracted brightness */ imgss=img[i]-sky[i]; /* Fill in this clump information. IMPORTANT NOTE: The Sky is not subtracted from the clump brightness or river, because later, we will subtract the river flux from the clump brightness and therefore we don't need to know the Sky for the clump brightness. */ ++thisclump[ CAREA ]; thisclump[ CGeoX ] += x; thisclump[ CGeoY ] += y; thisclump[ CGeoXX ] += sx * sx; thisclump[ CGeoYY ] += sy * sy; thisclump[ CGeoXY ] += sx * sy; thisclump[ CINHOSTID ] = clumps[i]; thisclump[ CHOSTOID ] = objects[i]; thisclump[ CBrightness ] += img[i]; thisclump[ CNoRiverBrightness ] += imgss; if( imgss > 0.0f ) { thisclump[ CPosBright ] += imgss; thisclump[ CFlxWhtX ] += imgss * x; thisclump[ CFlxWhtY ] += imgss * y; thisclump[ CFlxWhtXX ] += imgss * sx * sx; thisclump[ CFlxWhtYY ] += imgss * sy * sy; thisclump[ CFlxWhtXY ] += imgss * sx * sy; } } } /* We are on a detected region but not a clump (with a negative label). This region can be used to find properties like the river fluxs in the vicinity of clumps. */ else if (clumps[i]!=GAL_FITS_LONG_BLANK) /* We want to check the river pixels in each detection that has a clump. Recall that each detection can host more than one object. Since all the detection's pixels are given to one object, you can check if we are on an object or not with the clumps[i]<0 test. The process that keeps the labels of the clumps and their host object that have already been used for each river pixel in wngb wngb is inherited from the getclumpinfo function in NoiseChisel's clump.c. There is one big difference. When NoiseChisel was identifying the clumps, there were no `object's. The clumps were all within one detection. But here, the clumps can be separated by a one pixel thick river, but belong to different objects. So wngb has to keep two value for each neighboring clump: the object it belongs to and the clump within that object. */ if(clumps[i]<0 && p->oinfo[objects[i]*OCOLUMNS+ONCLUMPS] > 0.0f) { /* Make the preparations: */ ii=0; ind=&i; GAL_NEIGHBORS_FILL_8_ALLIMG; nf=(n=ngb)+numngb; memset(wngb, 0, sizeof(wngb)); /* Go over the neighbors and add the flux of this river pixel to a clump's information if it has not been added already. */ do if(clumps[*n]>0) { /* Go over wngb to see if this river pixel's value has been added to a segment or not. */ for(j=0;jfloatprecision, p->accuprecision}; int space[3]={p->intwidth, p->floatwidth, p->accuwidth}; /* Calculate the pixel area in arcseconds^2: */ pixarea=gal_wcs_pixel_area_arcsec2(p->wcs); /* First make the objects catalog, then the clumps catalog. */ for(p->obj0clump1=0;p->obj0clump1<2;++p->obj0clump1) { /* If no clumps image was provided, then ignore the clumps catalog. */ if(p->obj0clump1==1 && p->clumps==NULL) continue; /* Do the preparations for this round: */ p->intcounter=p->accucounter=p->curcol=0; p->name = p->obj0clump1 ? "clump" : "object"; p->icols = p->obj0clump1 ? CCOLUMNS : OCOLUMNS; p->info = p->obj0clump1 ? p->cinfo : p->oinfo; p->cat = p->obj0clump1 ? p->clumpcat : p->objcat; target = p->obj0clump1 ? MKCATCLUMP : MKCATOBJECT; p->filename = p->obj0clump1 ? p->ccatname : p->ocatname; cols = p->obj0clump1 ? p->clumpcols : p->objcols; p->numcols = p->obj0clump1 ? p->clumpncols : p->objncols; p->num = p->obj0clump1 ? p->numclumps : p->numobjects; /* Allocate the integer and accuracy arrays: */ errno=0; p->intcols=malloc(p->numcols*sizeof *p->intcols); if(p->intcols==NULL) error(EXIT_FAILURE, errno, "%zu bytes for intcols in makeoutput " "(mkcatalog.c)", p->numcols*sizeof *p->intcols); errno=0; p->accucols=malloc(p->numcols*sizeof *p->accucols); if(p->accucols==NULL) error(EXIT_FAILURE, errno, "%zu bytes for accucols in makeoutput " "(mkcatalog.c)", p->numcols*sizeof *p->accucols); /* Write the top of the comments: */ sprintf(comment, "# %s %s catalog.\n", SPACK_STRING, p->name); sprintf(p->line, "# %s started on %s", SPACK_NAME, ctime(&p->rawtime)); strcat(comment, p->line); if(gal_git_describe()) { sprintf(p->line, "# From commit %s\n", gal_git_describe()); strcat(comment, p->line); } /* Write the input files: */ strcat(comment, "#\n# Input files and information:\n" "# ----------------------------\n"); sprintf(p->line, "# Input %s (hdu: %s)\n", p->up.inputname, p->cp.hdu); strcat(comment, p->line); if(p->up.masknameset) { sprintf(p->line, "# Mask %s (hdu: %s)\n", p->up.maskname, p->up.mhdu); strcat(comment, p->line); } sprintf(p->line, "# Objects %s (hdu: %s)\n", p->up.objlabsname, p->up.objhdu); strcat(comment, p->line); if(p->up.clumplabsname) { sprintf(p->line, "# Clumps %s (hdu: %s)\n", p->up.clumplabsname, p->up.clumphdu); strcat(comment, p->line); } sprintf(p->line, "# Sky %s (hdu: %s)\n", p->up.skyname, p->up.skyhdu); strcat(comment, p->line); sprintf(p->line, "# Sky STD %s (hdu: %s)\n", p->up.stdname, p->up.stdhdu); strcat(comment, p->line); if(p->obj0clump1==0 && p->upmask) { sprintf(p->line, "# Upper limit magnitude mask %s (hdu: %s)\n", p->up.upmaskname, p->up.upmaskhdu); strcat(comment, p->line); } /* If a magnitude is also desired, print the zero point magnitude and the 5sigma magnitude: */ sprintf(p->line, "# "CATDESCRIPTLENGTH"%.3f\n", "Zero point magnitude:", p->zeropoint); strcat(comment, p->line); sprintf(tline, "Pixel %g sigma surface brightness (magnitude)", p->nsigmag); sprintf(p->line, "# "CATDESCRIPTLENGTH"%.3f\n", tline, -2.5f*log10(p->nsigmag*p->medstd)+p->zeropoint ); strcat(comment, p->line); sn = p->obj0clump1 ? p->clumpsn : p->detsn; if(!isnan(sn)) { sprintf(tline, "%s limiting Signal to noise ratio: ", p->obj0clump1 ? "Clump" : "Detection"); sprintf(p->line, "# "CATDESCRIPTLENGTH"%.3f\n", tline, sn); strcat(comment, p->line); if(p->obj0clump1==0) strcat(comment, "# (NOTE: limits above are for detections, not " "objects)\n"); } /* If cpscorr was used, report it: */ sprintf(p->line, "# "CATDESCRIPTLENGTH"%.3f\n", "Counts-per-second correction:", 1/p->cpscorr); strcat(comment, p->line); /* Report the area of each pixel in stradians: */ sprintf(p->line, "# "CATDESCRIPTLENGTH"%g\n", "Pixel area (arcsec^2)", pixarea); strcat(comment, p->line); /* if a threshold was used then report it: */ if(!isnan(p->threshold)) { sprintf(p->line, "# "CATDESCRIPTLENGTH"%g\n", "**IMPORTANT** " "Pixel threshold (multiple of local std)", p->threshold); strcat(comment, p->line); } /* If an upper limit was output then report its parameters: */ if(p->obj0clump1==0 && p->up.upperlimitmagset) { sprintf(p->line, "# "CATDESCRIPTLENGTH"%zu\n", "Number of upper " "limit magnitude samples", p->upnum); strcat(comment, p->line); sprintf(p->line, "# "CATDESCRIPTLENGTH"%zu\n", "Number of threads " "used for upper limit magnitude", p->cp.numthreads); strcat(comment, p->line); sprintf(p->line, "# "CATDESCRIPTLENGTH"%s\n", "Random number " "generator type for upper limit magnitude", gsl_rng_default->name); strcat(comment, p->line); sprintf(p->line, "# "CATDESCRIPTLENGTH"%zu\n", "Random number " "generator seed for upper limit magnitude", gsl_rng_default_seed); strcat(comment, p->line); sprintf(p->line, "# "CATDESCRIPTLENGTH"%.3f\n", "STD multiple for " "upper limit magnitude sigma-clip", p->upsclipmultip); strcat(comment, p->line); sprintf(p->line, "# "CATDESCRIPTLENGTH"%.3f\n", "STD accuracy " "to stop upper limit magnitude sigma-clip", p->upsclipaccu); strcat(comment, p->line); sprintf(p->line, "# "CATDESCRIPTLENGTH"%.3f\n", "Multiple of " "sigma for final upper limit magnitude", p->upnsigma); strcat(comment, p->line); } /* Prepare for printing the columns: */ strcat(comment, "#\n# Columns:\n# --------\n"); /* Fill the catalog array, in the end set the last elements in intcols and accucols to -1, so gal_txtarray_array_to_txt knows when to stop. */ for(p->curcol=0;p->curcolnumcols;++p->curcol) { col=cols[p->curcol]; switch(col) { case CATID: idcol(p); break; case CATHOSTOBJID: hostobj(p, 1); break; case CATIDINHOSTOBJ: hostobj(p, 0); break; case CATNUMCLUMPS: numclumps(p); break; case CATAREA: area(p, 0, 0); break; case CATCLUMPSAREA: area(p, 1, 0); break; case CATX: tmpcol = p->obj0clump1 ? CFlxWhtX : OFlxWhtX; position(p, tmpcol, target, MKCATWHTC, MKCATX); break; case CATY: tmpcol = p->obj0clump1 ? CFlxWhtY : OFlxWhtY; position(p, tmpcol, target, MKCATWHTC, MKCATY); break; case CATGEOX: tmpcol = p->obj0clump1 ? CGeoX : OGeoX; position(p, tmpcol, target, MKCATGEOC, MKCATX); break; case CATGEOY: tmpcol = p->obj0clump1 ? CGeoY : OGeoY; position(p, tmpcol, target, MKCATGEOC, MKCATY); break; case CATCLUMPSX: position(p, OFlxWhtCX, MKCATCINO, MKCATWHTC, MKCATX); break; case CATCLUMPSY: position(p, OFlxWhtCY, MKCATCINO, MKCATWHTC, MKCATY); break; case CATCLUMPSGEOX: position(p, OGeoCX, MKCATCINO, MKCATGEOC, MKCATX); break; case CATCLUMPSGEOY: position(p, OGeoCY, MKCATCINO, MKCATGEOC, MKCATY); break; case CATRA: tmpcol = p->obj0clump1 ? CFlxWhtRA : OFlxWhtRA; position(p, tmpcol, target, MKCATWHTC, MKCATRA); break; case CATDEC: tmpcol = p->obj0clump1 ? CFlxWhtDec : OFlxWhtDec; position(p, tmpcol, target, MKCATWHTC, MKCATDEC); break; case CATGEORA: tmpcol = p->obj0clump1 ? CGeoRA : OGeoRA; position(p, tmpcol, target, MKCATGEOC, MKCATRA); break; case CATGEODEC: tmpcol = p->obj0clump1 ? CGeoDec : OGeoDec; position(p, tmpcol, target, MKCATGEOC, MKCATDEC); break; case CATCLUMPSRA: position(p, OFlxWhtCRA, MKCATCINO, MKCATWHTC, MKCATRA); break; case CATCLUMPSDEC: position(p, OFlxWhtCDec, MKCATCINO, MKCATWHTC, MKCATDEC); break; case CATCLUMPSGEORA: position(p, OGeoCRA, MKCATCINO, MKCATGEOC, MKCATRA); break; case CATCLUMPSGEODEC: position(p, OGeoCDec, MKCATCINO, MKCATGEOC, MKCATDEC); break; case CATBRIGHTNESS: tmpcol = p->obj0clump1 ? CBrightness : OBrightness; brightnessmag(p, tmpcol, target, MKCATBRIGHT); break; case CATCLUMPSBRIGHTNESS: brightnessmag(p, OBrightnessC, MKCATCINO, MKCATBRIGHT); break; case CATNORIVERBRIGHTNESS: brightnessmag(p, CNoRiverBrightness, target, MKCATBRIGHT); break; case CATMAGNITUDE: tmpcol = p->obj0clump1 ? CBrightness : OBrightness; brightnessmag(p, tmpcol, target, MKCATMAG); break; case CATMAGNITUDEERR: sncol(p, 1, target); break; case CATCLUMPSMAGNITUDE: brightnessmag(p, OBrightnessC, MKCATCINO, MKCATMAG); break; case CATUPPERLIMITMAG: upperlimitcol(p); break; case CATRIVERAVE: brightnessmag(p, CRivAve, MKRIVERSSUR, MKCATBRIGHT); break; case CATRIVERNUM: area(p, 0, 1); break; case CATSN: sncol(p, 0, target); break; case CATSKY: skystd(p, p->obj0clump1 ? CSKY : OSKY); break; case CATSTD: skystd(p, p->obj0clump1 ? CSTD : OSTD); break; case CATSEMIMAJOR: case CATSEMIMINOR: case CATPOSITIONANGLE: case CATGEOSEMIMAJOR: case CATGEOSEMIMINOR: case CATGEOPOSITIONANGLE: secondordermoment(p, col, target); break; default: error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we " "can fix the problem. The value to cols[%zu] (%zu), is " "not recognized in makeoutput (mkcatalog.c)", PACKAGE_BUGREPORT, p->curcol, cols[p->curcol]); } sprintf(p->line, "# "CATDESCRIPTLENGTH"[%s]\n", p->description, p->unitp); strcat(comment, p->line); } p->intcols[p->intcounter]=p->accucols[p->accucounter]=-1; /* Write the catalog to file: */ gal_txtarray_array_to_txt(p->cat, p->num, p->numcols, comment, p->intcols, p->accucols, space, prec, 'f', p->filename); /* Clean up: */ free(p->intcols); free(p->accucols); } } /*********************************************************************/ /***************** Main function *******************/ /*********************************************************************/ void mkcatalog(struct mkcatalogparams *p) { /* Run through the data for the first time: */ firstpass(p); if(p->clumps) clumppass(p); /* Write the output: */ makeoutput(p); /* Clean up: */ free(p->oinfo); free(p->cinfo); } gnuastro-0.2.33-8a3b/bin/mkcatalog/args.h0000644000175000017500000005052212774160570014751 00000000000000/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef ARGS_H #define ARGS_H #include #include #include #include /**************************************************************/ /************** argp.h definitions ***************/ /**************************************************************/ /* Definition parameters for the argp: */ const char *argp_program_version=SPACK_STRING"\n"GAL_STRINGS_COPYRIGHT "\n\nWritten by Mohammad Akhlaghi"; const char *argp_program_bug_address=PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata"; const char doc[] = /* Before the list of options: */ GAL_STRINGS_TOP_HELP_INFO SPACK_NAME" will create a catalog from an input, labeled, and noise " "identification images.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /* Available letters for short options: f g k l u v w F G J L Q R U W X Y Z Number keys used: <= 541 Options with keys (second structure element) larger than 500 do not have a short version. */ static struct argp_option options[] = { { 0, 0, 0, 0, "Input:", 1 }, { "mask", 'M', "STR", 0, "Mask image file name.", 1 }, { "mhdu", 'H', "STR", 0, "Mask image header name or number.", 1 }, { "objlabs", 'O', "STR", 0, "Image specifying object labels.", 1 }, { "objhdu", 501, "STR", 0, "Object image header name or number.", 1 }, { "clumplabs", 'c', "STR", 0, "Image specifying clump labels.", 1 }, { "clumphdu", 502, "STR", 0, "Clumps image header name or number.", 1 }, { "skyfilename", 's', "STR", 0, "Sky value image.", 1 }, { "skyhdu", 503, "STR", 0, "Sky image header name or number.", 1 }, { "stdfilename", 't', "STR", 0, "Sky standard deviation image.", 1 }, { "stdhdu", 504, "STR", 0, "Sky STD image header name or number.", 1 }, { "zeropoint", 'z', "FLT", 0, "Image zeropoint magnitude.", 1 }, { "skysubtracted", 'E', 0, 0, "Input is already sky subtracted (for S/N).", 1 }, { "threshold", 'T', "FLT", 0, "Only values larger than this multiple of STD.", 1 }, { 0, 0, 0, 0, "Output:", 2 }, { "nsigmag", 521, "FLT", 0, "Multiple of Sky STD to report magnitude of.", 2 }, { "intwidth", 516, "INT", 0, "Width of integer columns.", 2 }, { "floatwidth", 517, "INT", 0, "Width of floating point columns.", 2 }, { "accuwidth", 518, "INT", 0, "Width of more accurate floating point columns.", 2 }, { "floatprecision", 519, "INT", 0, "Precision of floating point columns.", 2 }, { "accuprecision", 520, "INT", 0, "Precision of more accurate floating pnt. cols.", 2 }, { 0, 0, 0, 0, "Upper limit magnitude:", 3 }, { "upmask", 535, "STR", 0, "Mask image file name only for upper limit.", 3 }, { "upmaskhdu", 536, "STR", 0, "Upper limit mask image header name or number.", 3 }, { "upnum", 537, "INT", 0, "Number of randomly positioned samples.", 3 }, { "envseed", 540, 0, 0, "Random number generator info from environment.", 3 }, { "upsclipmultip", 538, "FLT", 0, "Sigma clipping multiple of std.", 3 }, { "upsclipaccu", 539, "FLT", 0, "Acceptable relative diff to stop clipping.", 3 }, { "upnsigma", 541, "FLT", 0, "Multiple of final sigma to use.", 3 }, { 0, 0, 0, 0, "Catalog columns:", 4 }, { "id", 'i', 0, 0, "Overall ID of this object or clump.", 4 }, { "hostobjid", 'j', 0, 0, "ID of object hosting this clump.", 4 }, { "idinhostobj", 'I', 0, 0, "ID of clump in host object.", 4 }, { "numclumps", 'C', 0, 0, "Number of clumps in this object.", 4 }, { "area", 'a', 0, 0, "Number of pixels.", 4 }, { "clumpsarea", 513, 0, 0, "Area of clumps in an object.", 4 }, { "x", 'x', 0, 0, "All obj. flux weighted center (first FITS axis).", 4 }, { "y", 'y', 0, 0, "All obj. flux weighted center (second FITS axis).", 4 }, { "geox", 522, 0, 0, "All obj. geometric center (first FITS axis).", 4 }, { "geoy", 523, 0, 0, "All obj. geometric center (second FITS axis).", 4 }, { "clumpsx", 507, 0, 0, "Clumps flux weighted center (first FITS axis).", 4 }, { "clumpsy", 508, 0, 0, "Clumps flux weighted center (second FITS axis).", 4 }, { "clumpsgeox", 524, 0, 0, "Clumps geometric center (first FITS axis).", 4 }, { "clumpsgeoy", 525, 0, 0, "Clumps geometric center (second FITS axis).", 4 }, { "ra", 'r', 0, 0, "All object flux weighted center right ascension.", 4 }, { "dec", 'd', 0, 0, "All object flux weighted center declination.", 4 }, { "geora", 526, 0, 0, "All object geometric center right ascension.", 4 }, { "geodec", 527, 0, 0, "All object geometric center declination.", 4 }, { "clumpsra", 509, 0, 0, "Clumps flux weighted center right ascension.", 4 }, { "clumpsdec", 510, 0, 0, "Clumps flux weighted center declination.", 4 }, { "clumpsgeora", 528, 0, 0, "Clumps geometric center right ascension.", 4 }, { "clumpsgeodec", 529, 0, 0, "Clumps geometric center declination.", 4 }, { "brightness", 'b', 0, 0, "Brightness (sum of pixel values).", 4 }, { "clumpbrightness", 511, 0, 0, "Brightness in clumps of an object.", 4 }, { "noriverbrightness", 533, 0, 0, "Sky (not river) subtracted clump brightness.", 4 }, { "magnitude", 'm', 0, 0, "Total magnitude.", 4 }, { "magnitudeerr", 'e', 0, 0, "Total magnitude error.", 4 }, { "clumpsmagnitude", 512, 0, 0, "Total magnitude of clumps in this object.", 4 }, { "upperlimitmag", 534, 0, 0, "Upper limit magnitude for each clump or object.", 4 }, { "riverave", 514, 0, 0, "Average river value surrounding this clump.", 4 }, { "rivernum", 515, 0, 0, "Number of river pixels surrounding this clump.", 4 }, { "sn", 'n', 0, 0, "Signal to noise ratio column.", 4 }, { "sky", 505, 0, 0, "Sky value.", 4 }, { "std", 506, 0, 0, "Sky standard deviation.", 4 }, { "semimajor", 'A', 0, 0, "Flux weighted Semi-major axis.", 4 }, { "semiminor", 'B', 0, 0, "Flux weighted Semi-minor axis.", 4 }, { "positionangle", 'p', 0, 0, "Flux weighted Position angle.", 4 }, { "geosemimajor", 530, 0, 0, "Flux weighted Semi-major axis.", 4 }, { "geosemiminor", 531, 0, 0, "Flux weighted Semi-minor axis.", 4 }, { "geopositionangle", 532, 0, 0, "Flux weighted Position angle.", 4 }, { 0, 0, 0, 0, "Operating modes:", -1 }, {0} }; /* Parse a single option: */ static error_t parse_opt(int key, char *arg, struct argp_state *state) { /* Save the arguments structure: */ struct mkcatalogparams *p = state->input; /* Set the pointer to the common parameters for all programs here: */ state->child_inputs[0]=&p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); switch(key) { /* Input: */ case 'M': gal_checkset_allocate_copy_set(arg, &p->up.maskname, &p->up.masknameset); break; case 'H': gal_checkset_allocate_copy_set(arg, &p->up.mhdu, &p->up.mhduset); break; case 'O': gal_checkset_allocate_copy_set(arg, &p->up.objlabsname, &p->up.objlabsnameset); break; case 501: gal_checkset_allocate_copy_set(arg, &p->up.objhdu, &p->up.objhduset); break; case 'c': gal_checkset_allocate_copy_set(arg, &p->up.clumplabsname, &p->up.clumplabsnameset); break; case 502: gal_checkset_allocate_copy_set(arg, &p->up.clumphdu, &p->up.clumphduset); break; case 's': gal_checkset_allocate_copy_set(arg, &p->up.skyname, &p->up.skynameset); break; case 503: gal_checkset_allocate_copy_set(arg, &p->up.skyhdu, &p->up.skyhduset); break; case 't': gal_checkset_allocate_copy_set(arg, &p->up.stdname, &p->up.stdnameset); break; case 504: gal_checkset_allocate_copy_set(arg, &p->up.stdhdu, &p->up.stdhduset); break; case 'z': gal_checkset_any_float(arg, &p->zeropoint, "zeropoint", key, SPACK, NULL, 0); p->up.zeropointset=1; break; case 'E': p->skysubtracted=1; p->up.skysubtractedset=1; break; case 'T': gal_checkset_any_double(arg, &p->threshold, "threshold", key, SPACK, NULL, 0); p->up.thresholdset=1; break; /* Output: */ case 521: gal_checkset_any_double(arg, &p->nsigmag, "nsigmag", key, SPACK, NULL, 0); p->up.nsigmagset=1; break; case 516: gal_checkset_int_l_zero(arg, &p->intwidth, "intwidth", key, SPACK, NULL, 0); p->up.intwidthset=1; break; case 517: gal_checkset_int_l_zero(arg, &p->floatwidth, "floatwidth", key, SPACK, NULL, 0); p->up.floatwidthset=1; break; case 518: gal_checkset_int_l_zero(arg, &p->accuwidth, "accuwidth", key, SPACK, NULL, 0); p->up.floatwidthset=1; break; case 519: gal_checkset_int_l_zero(arg, &p->floatprecision, "flatprecision", key, SPACK, NULL, 0); p->up.floatprecisionset=1; break; case 520: gal_checkset_int_l_zero(arg, &p->accuprecision, "accuprecision", key, SPACK, NULL, 0); p->up.accuprecisionset=1; break; /* Upper limit magnitude */ case 535: gal_checkset_allocate_copy_set(arg, &p->up.upmaskname, &p->up.upmasknameset); break; case 536: gal_checkset_allocate_copy_set(arg, &p->up.upmaskhdu, &p->up.upmaskhduset); break; case 537: gal_checkset_sizet_l_zero(arg, &p->upnum, "upnum", key, SPACK, NULL, 0); p->up.upnumset=1; break; case 540: p->envseed=1; p->up.envseedset=1; break; case 538: gal_checkset_float_l_0(arg, &p->upsclipmultip, "upsclipmultip", key, SPACK, NULL, 0); p->up.upsclipmultipset=1; break; case 539: gal_checkset_float_l_0_s_1(arg, &p->upsclipaccu, "upsclipaccu", key, SPACK, NULL, 0); p->up.upsclipaccuset=1; break; case 541: gal_checkset_float_l_0(arg, &p->upnsigma, "upnsigma", key, SPACK, NULL, 0); p->up.upnsigmaset=1; break; /* Catalog columns: */ case 'i': gal_linkedlist_add_to_sll(&p->allcolsll, CATID); p->up.idset=1; break; case 'j': gal_linkedlist_add_to_sll(&p->allcolsll, CATHOSTOBJID); p->up.hostobjidset=1; break; case 'I': gal_linkedlist_add_to_sll(&p->allcolsll, CATIDINHOSTOBJ); p->up.idinhostobjset=1; break; case 'C': gal_linkedlist_add_to_sll(&p->allcolsll, CATNUMCLUMPS); p->up.numclumpsset=1; break; case 'a': gal_linkedlist_add_to_sll(&p->allcolsll, CATAREA); p->up.areaset=1; break; case 513: gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSAREA); p->up.clumpsareaset=1; break; case 'x': gal_linkedlist_add_to_sll(&p->allcolsll, CATX); p->up.xset=1; break; case 'y': gal_linkedlist_add_to_sll(&p->allcolsll, CATY); p->up.yset=1; break; case 522: gal_linkedlist_add_to_sll(&p->allcolsll, CATGEOX); p->up.geoxset=1; break; case 523: gal_linkedlist_add_to_sll(&p->allcolsll, CATGEOY); p->up.geoyset=1; break; case 507: gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSX); p->up.clumpsxset=1; break; case 508: gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSY); p->up.clumpsyset=1; break; case 524: gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSGEOX); p->up.clumpsgeoxset=1; break; case 525: gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSGEOY); p->up.clumpsgeoyset=1; break; case 'r': gal_linkedlist_add_to_sll(&p->allcolsll, CATRA); p->up.raset=1; break; case 'd': gal_linkedlist_add_to_sll(&p->allcolsll, CATDEC); p->up.decset=1; break; case 526: gal_linkedlist_add_to_sll(&p->allcolsll, CATGEORA); p->up.georaset=1; break; case 527: gal_linkedlist_add_to_sll(&p->allcolsll, CATGEODEC); p->up.geodecset=1; break; case 509: gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSRA); p->up.clumpsraset=1; break; case 510: gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSDEC); p->up.clumpsdecset=1; break; case 528: gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSGEORA); p->up.clumpsgeoraset=1; break; case 529: gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSGEODEC); p->up.clumpsgeodecset=1; break; case 'b': gal_linkedlist_add_to_sll(&p->allcolsll, CATBRIGHTNESS); p->up.brightnessset=1; break; case 511: gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSBRIGHTNESS); p->up.clumpsbrightnessset=1; break; case 533: gal_linkedlist_add_to_sll(&p->allcolsll, CATNORIVERBRIGHTNESS); p->up.noriverbrightnessset=1; break; case 'm': gal_linkedlist_add_to_sll(&p->allcolsll, CATMAGNITUDE); p->up.magnitudeset=1; break; case 'e': gal_linkedlist_add_to_sll(&p->allcolsll, CATMAGNITUDEERR); p->up.magnitudeerrset=1; break; case 512: gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSMAGNITUDE); p->up.clumpsmagnitudeset=1; break; case 534: gal_linkedlist_add_to_sll(&p->allcolsll, CATUPPERLIMITMAG); p->up.upperlimitmagset=1; break; case 514: gal_linkedlist_add_to_sll(&p->allcolsll, CATRIVERAVE); p->up.riveraveset=1; break; case 515: gal_linkedlist_add_to_sll(&p->allcolsll, CATRIVERNUM); p->up.rivernumset=1; break; case 'n': gal_linkedlist_add_to_sll(&p->allcolsll, CATSN); p->up.snset=1; break; case 505: gal_linkedlist_add_to_sll(&p->allcolsll, CATSKY); p->up.skyset=1; break; case 506: gal_linkedlist_add_to_sll(&p->allcolsll, CATSTD); p->up.stdset=1; break; case 'A': gal_linkedlist_add_to_sll(&p->allcolsll, CATSEMIMAJOR); p->up.semimajorset=1; break; case 'B': gal_linkedlist_add_to_sll(&p->allcolsll, CATSEMIMINOR); p->up.semiminorset=1; break; case 'p': gal_linkedlist_add_to_sll(&p->allcolsll, CATPOSITIONANGLE); p->up.positionangleset=1; break; case 530: gal_linkedlist_add_to_sll(&p->allcolsll, CATGEOSEMIMAJOR); p->up.geosemimajorset=1; break; case 531: gal_linkedlist_add_to_sll(&p->allcolsll, CATGEOSEMIMINOR); p->up.geosemiminorset=1; break; case 532: gal_linkedlist_add_to_sll(&p->allcolsll, CATGEOPOSITIONANGLE); p->up.geopositionangleset=1; break; /* Operating modes: */ /* Read the non-option arguments: */ case ARGP_KEY_ARG: /* See what type of input value it is and put it in. */ if( gal_fits_name_is_fits(arg) ) { if(p->up.inputname) argp_error(state, "only one input image should be given"); else p->up.inputname=arg; } else argp_error(state, "%s is not a valid file type", arg); break; /* The command line options and arguments are finished. */ case ARGP_KEY_END: if(p->cp.setdirconf==0 && p->cp.setusrconf==0 && p->cp.printparams==0) { if(state->arg_num==0) argp_error(state, "no argument given"); if(p->up.inputname==NULL) argp_error(state, "no input FITS image(s) provided"); } break; default: return ARGP_ERR_UNKNOWN; } return 0; } /* Specify the children parsers: */ struct argp_child children[]= { {&commonargp, 0, NULL, 0}, {0, 0, 0, 0} }; /* Basic structure defining the whole argument reading process. */ static struct argp thisargp = {options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif gnuastro-0.2.33-8a3b/bin/mkcatalog/ui.h0000644000175000017500000000224512616616510014424 00000000000000/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef IMCROPUI_H #define IMCROPUI_H void setparams(int argc, char *argv[], struct mkcatalogparams *p); void freeandreport(struct mkcatalogparams *p, struct timeval *t1); #endif gnuastro-0.2.33-8a3b/bin/mkcatalog/ui.c0000644000175000017500000015431113001632540014407 00000000000000/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include /* From Gnulib. */ #include /* Includes time.h and sys/time.h */ #include #include #include #include "main.h" #include "ui.h" /* Needs main.h */ #include "args.h" /* Needs main.h, includes argp.h. */ /* Set the file names of the places where the default parameters are put. */ #define CONFIG_FILE SPACK CONF_POSTFIX #define SYSCONFIG_FILE SYSCONFIG_DIR "/" CONFIG_FILE #define USERCONFIG_FILEEND USERCONFIG_DIR CONFIG_FILE #define CURDIRCONFIG_FILE CURDIRCONFIG_DIR CONFIG_FILE /**************************************************************/ /************** Options and parameters ***************/ /**************************************************************/ void readconfig(char *filename, struct mkcatalogparams *p) { int yes; FILE *fp; size_t lineno=0, len=200; char *line, *name, *value; struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; char key='a'; /* Not used, just a place holder. */ /* When the file doesn't exist or can't be opened, it is ignored. It might be intentional, so there is no error. If a parameter is missing, it will be reported after all defaults are read. */ fp=fopen(filename, "r"); if (fp==NULL) return; /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); /* Read the tokens in the file: */ while(getline(&line, &len, fp) != -1) { /* Prepare the "name" and "value" strings, also set lineno. */ GAL_CONFIGFILES_START_READING_LINE; /* Inputs: */ if(strcmp(name, "hdu")==0) gal_checkset_allocate_copy_set(value, &cp->hdu, &cp->hduset); else if (strcmp(name, "mask")==0) gal_checkset_allocate_copy_set(value, &up->maskname, &up->masknameset); else if (strcmp(name, "mhdu")==0) gal_checkset_allocate_copy_set(value, &up->mhdu, &up->mhduset); else if (strcmp(name, "objlabs")==0) gal_checkset_allocate_copy_set(value, &up->objlabsname, &up->objlabsnameset); else if (strcmp(name, "objhdu")==0) gal_checkset_allocate_copy_set(value, &up->objhdu, &up->objhduset); else if (strcmp(name, "clumplabs")==0) gal_checkset_allocate_copy_set(value, &up->clumplabsname, &up->clumplabsnameset); else if (strcmp(name, "clumphdu")==0) gal_checkset_allocate_copy_set(value, &up->clumphdu, &up->clumphduset); else if (strcmp(name, "skyfilename")==0) gal_checkset_allocate_copy_set(value, &up->skyname, &up->skynameset); else if (strcmp(name, "skyhdu")==0) gal_checkset_allocate_copy_set(value, &up->skyhdu, &up->skyhduset); else if (strcmp(name, "stdfilename")==0) gal_checkset_allocate_copy_set(value, &up->stdname, &up->stdnameset); else if (strcmp(name, "stdhdu")==0) gal_checkset_allocate_copy_set(value, &up->stdhdu, &up->stdhduset); else if (strcmp(name, "zeropoint")==0) { if(up->zeropointset) continue; gal_checkset_any_float(value, &p->zeropoint, name, key, SPACK, filename, lineno); up->zeropointset=1; } else if (strcmp(name, "skysubtracted")==0) { if(up->skysubtractedset) continue; gal_checkset_int_zero_or_one(value, &p->skysubtracted, name, key, SPACK, filename, lineno); up->skysubtractedset=1; } else if(strcmp(name, "threshold")==0) { if(up->thresholdset) continue; gal_checkset_any_double(value, &p->threshold, name, key, SPACK, filename, lineno); up->thresholdset=1; } /* Outputs */ else if(strcmp(name, "output")==0) gal_checkset_allocate_copy_set(value, &cp->output, &cp->outputset); else if(strcmp(name, "nsigmag")==0) { if(up->nsigmagset) continue; gal_checkset_any_double(value, &p->nsigmag, name, key, SPACK, filename, lineno); up->nsigmagset=1; } else if(strcmp(name, "intwidth")==0) { if(up->intwidthset) continue; gal_checkset_int_l_zero(value, &p->intwidth, name, key, SPACK, filename, lineno); up->intwidthset=1; } else if(strcmp(name, "floatwidth")==0) { if(up->floatwidthset) continue; gal_checkset_int_l_zero(value, &p->floatwidth, name, key, SPACK, filename, lineno); up->floatwidthset=1; } else if(strcmp(name, "accuwidth")==0) { if(up->accuwidthset) continue; gal_checkset_int_l_zero(value, &p->accuwidth, name, key, SPACK, filename, lineno); up->accuwidthset=1; } else if(strcmp(name, "floatprecision")==0) { if(up->floatprecisionset) continue; gal_checkset_int_l_zero(value, &p->floatprecision, name, key, SPACK, filename, lineno); up->floatprecisionset=1; } else if(strcmp(name, "accuprecision")==0) { if(up->accuprecisionset) continue; gal_checkset_int_l_zero(value, &p->accuprecision, name, key, SPACK, filename, lineno); up->accuprecisionset=1; } /* Upper limit magnitude */ else if (strcmp(name, "upmaskname")==0) gal_checkset_allocate_copy_set(value, &up->upmaskname, &up->upmasknameset); else if (strcmp(name, "upmaskhdu")==0) gal_checkset_allocate_copy_set(value, &up->upmaskhdu, &up->upmaskhduset); else if(strcmp(name, "upnum")==0) { if(up->upnumset) continue; gal_checkset_sizet_l_zero(value, &p->upnum, name, key, SPACK, filename, lineno); up->upnumset=1; } else if(strcmp(name, "envseed")==0) { if(up->envseedset) continue; gal_checkset_int_zero_or_one(value, &p->envseed, name, key, SPACK, filename, lineno); up->envseedset=1; } else if(strcmp(name, "upsclipmultip")==0) { if(up->upsclipmultipset) continue; gal_checkset_float_l_0(value, &p->upsclipmultip, name, key, SPACK, filename, lineno); up->upsclipmultipset=1; } else if(strcmp(name, "upsclipaccu")==0) { if(up->upsclipaccuset) continue; gal_checkset_float_l_0_s_1(value, &p->upsclipaccu, name, key, SPACK, filename, lineno); up->upsclipaccuset=1; } else if(strcmp(name, "upnsigma")==0) { if(up->upnsigmaset) continue; gal_checkset_float_l_0(value, &p->upnsigma, name, key, SPACK, filename, lineno); up->upnsigmaset=1; } /* Catalog columns */ else if(strcmp(name, "id")==0) { if(up->idset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATID); up->idset=1; } else if(strcmp(name, "hostobjid")==0) { if(up->hostobjidset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATHOSTOBJID); up->hostobjidset=1; } else if(strcmp(name, "idinhostobj")==0) { if(up->idinhostobjset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATIDINHOSTOBJ); up->idinhostobjset=1; } else if(strcmp(name, "numclumps")==0) { if(up->numclumpsset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATNUMCLUMPS); up->numclumpsset=1; } else if(strcmp(name, "area")==0) { if(up->areaset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATAREA); up->areaset=1; } else if(strcmp(name, "clumpsarea")==0) { if(up->clumpsareaset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSAREA); up->clumpsareaset=1; } else if(strcmp(name, "x")==0) { if(up->xset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATX); up->xset=1; } else if(strcmp(name, "y")==0) { if(up->yset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATY); up->yset=1; } else if(strcmp(name, "geox")==0) { if(up->geoxset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATGEOX); up->geoxset=1; } else if(strcmp(name, "geoy")==0) { if(up->geoyset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATGEOY); up->geoyset=1; } else if(strcmp(name, "clumpsx")==0) { if(up->clumpsxset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSX); up->clumpsxset=1; } else if(strcmp(name, "clumpsy")==0) { if(up->clumpsyset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSY); up->clumpsyset=1; } else if(strcmp(name, "clumpsgeox")==0) { if(up->clumpsgeoxset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSGEOX); up->clumpsgeoxset=1; } else if(strcmp(name, "clumpsgeoy")==0) { if(up->clumpsgeoyset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSGEOY); up->clumpsgeoyset=1; } else if(strcmp(name, "ra")==0) { if(up->raset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATRA); up->raset=1; } else if(strcmp(name, "dec")==0) { if(up->decset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATDEC); up->decset=1; } else if(strcmp(name, "geora")==0) { if(up->georaset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATGEORA); up->georaset=1; } else if(strcmp(name, "geodec")==0) { if(up->geodecset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATGEODEC); up->geodecset=1; } else if(strcmp(name, "clumpsra")==0) { if(up->clumpsraset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSRA); up->clumpsraset=1; } else if(strcmp(name, "clumpsdec")==0) { if(up->clumpsdecset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSDEC); up->clumpsdecset=1; } else if(strcmp(name, "clumpsgeora")==0) { if(up->clumpsgeoraset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSGEORA); up->clumpsgeoraset=1; } else if(strcmp(name, "clumpsgeodec")==0) { if(up->clumpsgeodecset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSGEODEC); up->clumpsgeodecset=1; } else if(strcmp(name, "brightness")==0) { if(up->brightnessset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATBRIGHTNESS); up->brightnessset=1; } else if(strcmp(name, "clumpsbrightness")==0) { if(up->clumpsbrightnessset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSBRIGHTNESS); p->up.clumpsbrightnessset=1; } else if(strcmp(name, "noriverbrightness")==0) { if(up->noriverbrightnessset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATNORIVERBRIGHTNESS); p->up.noriverbrightnessset=1; } else if(strcmp(name, "magnitude")==0) { if(up->magnitudeset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATMAGNITUDE); up->magnitudeset=1; } else if(strcmp(name, "magnitudeerr")==0) { if(up->magnitudeerrset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATMAGNITUDEERR); up->magnitudeerrset=1; } else if(strcmp(name, "clumpsmagnitude")==0) { if(up->clumpsmagnitudeset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATCLUMPSMAGNITUDE); up->clumpsmagnitudeset=1; } else if(strcmp(name, "upperlimitmag")==0) { if(up->upperlimitmagset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATUPPERLIMITMAG); up->upperlimitmagset=1; } else if(strcmp(name, "riverave")==0) { if(up->riveraveset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATRIVERAVE); up->riveraveset=1; } else if(strcmp(name, "rivernum")==0) { if(up->rivernumset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATRIVERNUM); up->rivernumset=1; } else if(strcmp(name, "sn")==0) { if(up->snset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATSN); up->snset=1; } else if(strcmp(name, "sky")==0) { if(up->skyset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATSKY); up->skyset=1; } else if(strcmp(name, "std")==0) { if(up->stdset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATSTD); up->stdset=1; } else if(strcmp(name, "semimajor")==0) { if(up->semimajorset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATSEMIMAJOR); up->semimajorset=1; } else if(strcmp(name, "semiminor")==0) { if(up->semiminorset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATSEMIMINOR); up->semiminorset=1; } else if(strcmp(name, "positionangle")==0) { if(up->positionangleset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATPOSITIONANGLE); up->positionangleset=1; } else if(strcmp(name, "geosemimajor")==0) { if(up->geosemimajorset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATGEOSEMIMAJOR); up->geosemimajorset=1; } else if(strcmp(name, "geosemiminor")==0) { if(up->geosemiminorset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATGEOSEMIMINOR); up->geosemiminorset=1; } else if(strcmp(name, "geopositionangle")==0) { if(up->geopositionangleset) continue; gal_checkset_int_zero_or_one(value, &yes, name, key, SPACK, filename, lineno); if(!yes) continue; gal_linkedlist_add_to_sll(&p->allcolsll, CATGEOPOSITIONANGLE); up->geopositionangleset=1; } /* Operating modes */ /* Read options common to all programs */ GAL_CONFIGFILES_READ_COMMONOPTIONS_FROM_CONF else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s` not recognized.\n", name); } free(line); fclose(fp); } void printvalues(FILE *fp, struct mkcatalogparams *p) { int i; struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; /* Print all the options that are set. Separate each group with a commented line explaining the options in that group. */ fprintf(fp, "\n# Input image:\n"); if(cp->hduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("hdu", cp->hdu); if(up->masknameset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("mask", up->maskname); if(up->mhduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("mhdu", up->mhdu); if(up->objlabsnameset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("objlabs", up->objlabsname); if(up->objhduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("objhdu", up->objhdu); if(up->clumplabsnameset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("clumplabs", up->clumplabsname); if(up->clumphduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("clumphdu", up->clumphdu); if(up->skynameset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("skyfilename", up->skyname); if(up->skyhduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("skyhdu", up->skyhdu); if(up->stdnameset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("stdfilename", up->stdname); if(up->stdhduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("stdhdu", up->stdhdu); if(up->zeropointset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "zeropoint", p->zeropoint); if(up->skysubtractedset) fprintf(fp, CONF_SHOWFMT"%d\n", "skysubtracted", p->skysubtracted); if(up->thresholdset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "threshold", p->threshold); /* Output: */ fprintf(fp, "\n# Output:\n"); if(cp->outputset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("output", cp->output); if(up->nsigmagset) fprintf(fp, CONF_SHOWFMT"%g\n", "nsigmag", p->nsigmag); if(up->intwidthset) fprintf(fp, CONF_SHOWFMT"%d\n", "intwidth", p->intwidth); if(up->floatwidthset) fprintf(fp, CONF_SHOWFMT"%d\n", "floatwidth", p->floatwidth); if(up->accuwidthset) fprintf(fp, CONF_SHOWFMT"%d\n", "accuwidth", p->accuwidth); if(up->floatprecisionset) fprintf(fp, CONF_SHOWFMT"%d\n", "floatprecision", p->floatprecision); if(up->accuprecisionset) fprintf(fp, CONF_SHOWFMT"%d\n", "accuprecision", p->accuprecision); /* Upper limit magnitude */ fprintf(fp, "\n# Upper limit magnitude:\n"); if(up->upmasknameset) fprintf(fp, CONF_SHOWFMT"%s\n", "upmaskname", up->upmaskname); if(up->upmaskhduset) fprintf(fp, CONF_SHOWFMT"%s\n", "upmaskhdu", up->upmaskhdu); if(up->upnumset) fprintf(fp, CONF_SHOWFMT"%zu\n", "upnum", p->upnum); if(up->envseedset) fprintf(fp, CONF_SHOWFMT"%d\n", "envseed", p->envseed); if(up->upsclipmultipset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "upsclipmultip", p->upsclipmultip); if(up->upsclipaccuset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "upsclipaccu", p->upsclipaccu); if(up->upnsigmaset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "upnsigma", p->upnsigma); /* Catalog columns, since order is important. Notice that they have to be printed in opposite order (because of the way they are read through a simple linked list). */ fprintf(fp, "\n# Catalog columns:\n"); for(i=p->allncols-1;i>=0;--i) switch(p->allcols[i]) { case CATID: fprintf(fp, CONF_SHOWFMT"%d\n", "id", 1); break; case CATHOSTOBJID: fprintf(fp, CONF_SHOWFMT"%d\n", "hostobjid", 1); break; case CATIDINHOSTOBJ: fprintf(fp, CONF_SHOWFMT"%d\n", "idinhostobj", 1); break; case CATNUMCLUMPS: fprintf(fp, CONF_SHOWFMT"%d\n", "numclumps", 1); break; case CATAREA: fprintf(fp, CONF_SHOWFMT"%d\n", "area", 1); break; case CATCLUMPSAREA: fprintf(fp, CONF_SHOWFMT"%d\n", "clumpsarea", 1); break; case CATX: fprintf(fp, CONF_SHOWFMT"%d\n", "x", 1); break; case CATY: fprintf(fp, CONF_SHOWFMT"%d\n", "y", 1); break; case CATGEOX: fprintf(fp, CONF_SHOWFMT"%d\n", "x", 1); break; case CATGEOY: fprintf(fp, CONF_SHOWFMT"%d\n", "y", 1); break; case CATCLUMPSX: fprintf(fp, CONF_SHOWFMT"%d\n", "clumpsx", 1); break; case CATCLUMPSY: fprintf(fp, CONF_SHOWFMT"%d\n", "clumpsy", 1); break; case CATCLUMPSGEOX: fprintf(fp, CONF_SHOWFMT"%d\n", "clumpsgeox", 1); break; case CATCLUMPSGEOY: fprintf(fp, CONF_SHOWFMT"%d\n", "clumpsgeoy", 1); break; case CATRA: fprintf(fp, CONF_SHOWFMT"%d\n", "ra", 1); break; case CATDEC: fprintf(fp, CONF_SHOWFMT"%d\n", "dec", 1); break; case CATGEORA: fprintf(fp, CONF_SHOWFMT"%d\n", "geora", 1); break; case CATGEODEC: fprintf(fp, CONF_SHOWFMT"%d\n", "geodec", 1); break; case CATCLUMPSRA: fprintf(fp, CONF_SHOWFMT"%d\n", "clumpsra", 1); break; case CATCLUMPSDEC: fprintf(fp, CONF_SHOWFMT"%d\n", "clumpsdec", 1); break; case CATCLUMPSGEORA: fprintf(fp, CONF_SHOWFMT"%d\n", "clumpsgeora", 1); break; case CATCLUMPSGEODEC: fprintf(fp, CONF_SHOWFMT"%d\n", "clumpsgeodec", 1); break; case CATBRIGHTNESS: fprintf(fp, CONF_SHOWFMT"%d\n", "brightness", 1); break; case CATCLUMPSBRIGHTNESS: fprintf(fp, CONF_SHOWFMT"%d\n", "clumpsbrightness", 1); break; case CATUPPERLIMITMAG: fprintf(fp, CONF_SHOWFMT"%d\n", "upperlimitmag", 1); break; case CATNORIVERBRIGHTNESS: fprintf(fp, CONF_SHOWFMT"%d\n", "noriverbrightness", 1); break; case CATMAGNITUDE: fprintf(fp, CONF_SHOWFMT"%d\n", "magnitude", 1); break; case CATMAGNITUDEERR: fprintf(fp, CONF_SHOWFMT"%d\n", "magnitudeerr", 1); break; case CATCLUMPSMAGNITUDE: fprintf(fp, CONF_SHOWFMT"%d\n", "clumpsmagnitude", 1); break; case CATRIVERAVE: fprintf(fp, CONF_SHOWFMT"%d\n", "riverave", 1); break; case CATRIVERNUM: fprintf(fp, CONF_SHOWFMT"%d\n", "rivernum", 1); break; case CATSN: fprintf(fp, CONF_SHOWFMT"%d\n", "sn", 1); break; case CATSKY: fprintf(fp, CONF_SHOWFMT"%d\n", "sky", 1); break; case CATSTD: fprintf(fp, CONF_SHOWFMT"%d\n", "std", 1); break; case CATSEMIMAJOR: fprintf(fp, CONF_SHOWFMT"%d\n", "semimajor", 1); break; case CATSEMIMINOR: fprintf(fp, CONF_SHOWFMT"%d\n", "semiminor", 1); break; case CATPOSITIONANGLE: fprintf(fp, CONF_SHOWFMT"%d\n", "positionangle", 1); break; case CATGEOSEMIMAJOR: fprintf(fp, CONF_SHOWFMT"%d\n", "geosemimajor", 1); break; case CATGEOSEMIMINOR: fprintf(fp, CONF_SHOWFMT"%d\n", "geosemiminor", 1); break; case CATGEOPOSITIONANGLE: fprintf(fp, CONF_SHOWFMT"%d\n", "geopositionangle", 1); break; default: error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we can " "fix the problem. For some reason p->allcols[%d] is given " "the value %zu which is not recognized in printvalues " "(ui.c)", PACKAGE_BUGREPORT, i, p->allcols[i]); } /* For the operating mode, first put the macro to print the common options, then the (possible options particular to this program). */ fprintf(fp, "\n# Operating mode:\n"); GAL_CONFIGFILES_PRINT_COMMONOPTIONS; } /* Note that numthreads will be used automatically based on the configure time. */ void checkifset(struct mkcatalogparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; int intro=0; if(cp->hduset==0) GAL_CONFIGFILES_REPORT_NOTSET("hdu"); if(up->objhduset==0) GAL_CONFIGFILES_REPORT_NOTSET("objhdu"); if(up->clumphduset==0) GAL_CONFIGFILES_REPORT_NOTSET("clumphdu"); if(up->skyhduset==0) GAL_CONFIGFILES_REPORT_NOTSET("skyhdu"); if(up->stdhduset==0) GAL_CONFIGFILES_REPORT_NOTSET("stdhdu"); if(up->zeropointset==0) GAL_CONFIGFILES_REPORT_NOTSET("zeropoint"); if(up->skysubtractedset==0) GAL_CONFIGFILES_REPORT_NOTSET("skysubtracted"); /* Output: */ if(up->nsigmagset==0) GAL_CONFIGFILES_REPORT_NOTSET("nsigmag"); if(up->intwidthset==0) GAL_CONFIGFILES_REPORT_NOTSET("intwidth"); if(up->floatwidthset==0) GAL_CONFIGFILES_REPORT_NOTSET("floatwidth"); if(up->accuwidthset==0) GAL_CONFIGFILES_REPORT_NOTSET("accuwidth"); if(up->floatprecisionset==0) GAL_CONFIGFILES_REPORT_NOTSET("floatprecision"); if(up->accuprecisionset==0) GAL_CONFIGFILES_REPORT_NOTSET("accuprecision"); /* Upper limit magnitude. */ if(p->up.upperlimitmagset) { if(p->up.upnumset==0) GAL_CONFIGFILES_REPORT_NOTSET("upnum"); if(p->up.upsclipmultipset==0) GAL_CONFIGFILES_REPORT_NOTSET("upsclipmultip"); if(p->up.upsclipaccuset==0) GAL_CONFIGFILES_REPORT_NOTSET("upsclipaccu"); if(p->up.upnsigmaset==0) GAL_CONFIGFILES_REPORT_NOTSET("upnsigma"); } GAL_CONFIGFILES_END_OF_NOTSET_REPORT; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ void sanitycheck(struct mkcatalogparams *p) { struct uiparams *up=&p->up; struct gal_fits_key keys[1]; struct gal_commonparams *cp=&p->cp; /* Make sure the input file exists. */ gal_checkset_check_file(up->inputname); /* Set the names of the files. */ gal_fits_file_or_ext_name(up->inputname, p->cp.hdu, up->masknameset, &up->maskname, up->mhdu, up->mhduset, "mask"); gal_fits_file_or_ext_name(up->inputname, p->cp.hdu, up->objlabsnameset, &up->objlabsname, up->objhdu, up->objhduset, "object labels"); gal_fits_file_or_ext_name(up->inputname, p->cp.hdu, up->skynameset, &up->skyname, up->skyhdu, up->skyhduset, "sky value image"); gal_fits_file_or_ext_name(up->inputname, p->cp.hdu, up->stdnameset, &up->stdname, up->stdhdu, up->stdhduset, "sky standard deviation"); /* The WCLUMPS (with-clumps) keyword in the object HDU says that there is also a clumps image accompaning the object image. If it exists and its value is `yes' (not case sensitive), then set the image name to the proper string. Otherwise, set the image name to NULL, so future functions can check. */ keys[0].str[0]='\0'; keys[0].datatype=TSTRING; keys[0].keyname="WCLUMPS"; gal_fits_read_keywords(up->objlabsname, up->objhdu, keys, 1); if(strcasecmp(keys[0].str, "yes")) up->clumplabsname=NULL; else gal_fits_file_or_ext_name(up->inputname, p->cp.hdu, up->clumplabsnameset, &up->clumplabsname, up->clumphdu, up->clumphduset, "clump labels"); /* When the RA and Dec are needed, make sure that the X and Y columns and the RA and Dec columns in the information array are immediately after each other and in this order. This is not set by the user, but by the programmer. Nevertheless, it is a very important issue to check. Since the enum values are constants, the compiler will know immediately and stop. NOTE: the information array is separate from the output array */ if(up->raset || up->decset) { if( OFlxWhtX!=OFlxWhtY-1 || OFlxWhtRA!=OFlxWhtDec-1 ) error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we can " "fix the problem. X(%d) and Y(%d), or Ra(%d) and Dec(%d) " "columns in the information array are not immediately " "after each other", PACKAGE_BUGREPORT, OFlxWhtX, OFlxWhtY, OFlxWhtRA, OFlxWhtDec); } /* Set the output names, based on if the output is set or not. */ gal_checkset_automatic_output(cp->outputset ? cp->output : up->inputname, up->clumplabsname ? "_o.txt" : ".txt", cp->outputset ? 0 : p->cp.removedirinfo, p->cp.dontdelete, &p->ocatname); if(up->clumplabsname) gal_checkset_automatic_output(cp->outputset ? cp->output : up->inputname, "_c.txt", cp->outputset ? 0 : p->cp.removedirinfo, p->cp.dontdelete, &p->ccatname); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ void checksetlong(struct mkcatalogparams *p, char *filename, char *hdu, long **array) { size_t s0, s1; int bitpix, anyblank; /* Read the file: */ gal_fits_file_to_long(filename, hdu, array, &bitpix, &anyblank, &s0, &s1); /* Make sure it has an integer type. */ if(bitpix==FLOAT_IMG || bitpix==DOUBLE_IMG) error(EXIT_FAILURE, 0, "the labels image can be any integer type " "(BITPIX). However, %s (hdu: %s) is a %s precision floating " "point image", filename, hdu, bitpix==FLOAT_IMG ? "single" : "double"); /* Make sure it is the same size as the input image. */ if(s0!=p->s0 || s1!=p->s1) error(EXIT_FAILURE, 0, "%s (hdu: %s) is %zu x %zu pixels while the " "%s (hdu: %s) is %zu x %zu. The images should have the same " "size", filename, hdu, s1, s0, p->up.inputname, p->cp.hdu, p->s1, p->s0); } void checksetfloat(struct mkcatalogparams *p, char *filename, char *hdu, float **array) { size_t s0, s1; int bitpix, anyblank; /* Read the array: */ gal_fits_file_to_float(filename, NULL, hdu, NULL, array, &bitpix, &anyblank, &s0, &s1); /* Make sure it has no blank pixels. if(anyblank) error(EXIT_FAILURE, 0, "the Sky and Sky standard deviation images " "should not have any blank values. %s (hdu: %s) has blank " "pixels", filename, hdu); */ /* Make sure it has the same size as the image. */ if(s0!=p->s0 || s1!=p->s1) error(EXIT_FAILURE, 0, "%s (hdu: %s) is %zu x %zu pixels while the " "%s (hdu: %s) is %zu x %zu. The images should have the same " "size", filename, hdu, s1, s0, p->up.inputname, p->cp.hdu, p->s1, p->s0); } /* Read the necessary keywords and if they aren't present do the appropriate action. */ void readkeywords(struct mkcatalogparams *p) { long numobjects; size_t size=p->s0*p->s1; struct uiparams *up=&p->up; struct gal_fits_key keys[2]; /* Read keywords from the standard deviation image: */ keys[0].keyname="MINSTD"; keys[0].datatype=TFLOAT; keys[1].keyname="MEDSTD"; keys[1].datatype=TFLOAT; gal_fits_read_keywords(up->stdname, up->stdhdu, keys, 2); /* The minimum standard deviation value. */ if(keys[0].status) gal_statistics_float_min(p->std, size, &p->minstd); else p->minstd=keys[0].f; p->cpscorr = p->minstd>1 ? 1.0f : p->minstd; /* Median standard deviation value (only necessary in catalog comments). */ if(keys[1].status) { p->medstd=gal_statistics_median(p->std, size); fprintf(stderr, "Warning: Could not find the MEDSTD keyword in %s " "(hdu: %s). The median standard deviation is thus found on " "the (interpolated) standard deviation image. NoiseChisel " "finds the median before interpolation, so the reported value " "in the final catalog will not be accurate (will depend on " "how many meshs were blank and their spatial position " "relative to the non-blank ones.", up->stdname, up->stdhdu); } else p->medstd=keys[1].f; /* Read the keywords from the objects image: */ keys[0].keyname="DETSN"; keys[0].datatype=TDOUBLE; keys[1].keyname="NOBJS"; keys[1].datatype=TLONG; gal_fits_read_keywords(up->objlabsname, up->objhdu, keys, 2); /* If DETSN is not given, there is no way we can calculate it here, so we will just set it to NaN to check and not report in the end. */ p->detsn = keys[0].status ? NAN : keys[0].d; /* Read the total number of objects. */ if(keys[1].status) { gal_statistics_long_non_blank_max(p->objects, size, &numobjects, GAL_FITS_LONG_BLANK); p->numobjects=numobjects; } else p->numobjects=keys[1].l; /* Read the clumps information if it is necessary. Note that unlike finding the number of objects, finding the number of clumps is not an easy process, since the clumps of each object start with a label of one. So if the number of clumps is not given, we have to abort. For now, is up to the program that built the clumps to give the total number, later we can take a procedure to find them (for example first only taking the positive labels (that are clumps) and making a binary image, then running the connected component algorithm to find the number of clumps in the image.*/ if(up->clumplabsname) { keys[0].keyname="CLUMPSN"; keys[1].keyname="NCLUMPS"; gal_fits_read_keywords(up->clumplabsname, up->clumphdu, keys, 2); p->clumpsn = keys[0].status ? NAN : keys[0].d; if(keys[1].status) error(EXIT_FAILURE, 0, "couldn't find NCLUMPS in the header of " "%s (hdu: %s).", up->clumplabsname, up->clumphdu); else p->numclumps=keys[1].l; } } void preparearrays(struct mkcatalogparams *p) { size_t i; int bitpix, anyblank; /* Prepare the columns and allocate the p->objcols and p->clumpcols arrays to keep the macros of what output they should keep. */ gal_linkedlist_sll_to_array(p->allcolsll, &p->allcols, &p->allncols, 0); if(p->allncols==0) error(EXIT_FAILURE, 0, "no columns specified for output"); errno=0; p->objcols=malloc(p->allncols*sizeof *p->objcols); if(p->objcols==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->objcols in " "preprarearrays (ui.c)", p->allncols*sizeof *p->objcols); errno=0; p->clumpcols=malloc(p->allncols*sizeof *p->clumpcols); if(p->clumpcols==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->clumpcols in " "preprarearrays (ui.c)", p->allncols*sizeof *p->clumpcols); /* Put all the input columns into the object or clumps columns and count how many columns each should have. */ p->objncols=p->clumpncols=0; for(i=0;iallncols;++i) { switch(p->allcols[i]) { case CATID: p->objcols[p->objncols++]=p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATHOSTOBJID: p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATIDINHOSTOBJ: p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATNUMCLUMPS: p->objcols[p->objncols++] = p->allcols[i]; break; case CATAREA: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATCLUMPSAREA: p->objcols[p->objncols++] = p->allcols[i]; break; case CATX: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATY: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATGEOX: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATGEOY: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATCLUMPSX: p->objcols[p->objncols++] = p->allcols[i]; break; case CATCLUMPSY: p->objcols[p->objncols++] = p->allcols[i]; break; case CATCLUMPSGEOX: p->objcols[p->objncols++] = p->allcols[i]; break; case CATCLUMPSGEOY: p->objcols[p->objncols++] = p->allcols[i]; break; case CATRA: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATDEC: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATGEORA: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATGEODEC: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATCLUMPSRA: p->objcols[p->objncols++] = p->allcols[i]; break; case CATCLUMPSDEC: p->objcols[p->objncols++] = p->allcols[i]; break; case CATCLUMPSGEORA: p->objcols[p->objncols++] = p->allcols[i]; break; case CATCLUMPSGEODEC: p->objcols[p->objncols++] = p->allcols[i]; break; case CATBRIGHTNESS: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATCLUMPSBRIGHTNESS: p->objcols[p->objncols++] = p->allcols[i]; break; case CATUPPERLIMITMAG: p->objcols[p->objncols++] = p->allcols[i]; break; case CATNORIVERBRIGHTNESS: p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATMAGNITUDE: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATMAGNITUDEERR: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATCLUMPSMAGNITUDE: p->objcols[p->objncols++] = p->allcols[i]; break; case CATRIVERAVE: p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATRIVERNUM: p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATSN: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATSKY: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATSTD: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATSEMIMAJOR: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATSEMIMINOR: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATPOSITIONANGLE: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATGEOSEMIMAJOR: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATGEOSEMIMINOR: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; case CATGEOPOSITIONANGLE: p->objcols[p->objncols++] = p->allcols[i]; p->clumpcols[p->clumpncols++] = p->allcols[i]; break; default: error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we " "can fix the problem. For some reason p->allcols[%zu] " "is given the value %zu which is not recognized in " "preparearrays (ui.c)", PACKAGE_BUGREPORT, i, p->allcols[i]); } } /* Read the input image. Note that after this step, everything depends on having an input filename. If the user just wants to check the parameters, there is no input file name. */ if(p->up.inputname) { gal_fits_file_to_float(p->up.inputname, p->up.maskname, p->cp.hdu, p->up.mhdu, &p->img, &bitpix, &anyblank, &p->s0, &p->s1); gal_fits_read_wcs(p->up.inputname, p->cp.hdu, 0, 0, &p->nwcs, &p->wcs); /* Read and check the object, sky and skystd HDUs. Note that the clumps image is only used when the objects image says a clumps image exists. */ checksetfloat(p, p->up.skyname, p->up.skyhdu, &p->sky); checksetfloat(p, p->up.stdname, p->up.stdhdu, &p->std); checksetlong(p, p->up.objlabsname, p->up.objhdu, &p->objects); if(p->up.clumplabsname) checksetlong(p, p->up.clumplabsname, p->up.clumphdu, &p->clumps); else p->clumps=NULL; if(p->up.upmasknameset) checksetlong(p, p->up.upmaskname, p->up.upmaskhdu, &p->upmask); else p->upmask=NULL; /* Read the necessary keywords. */ readkeywords(p); /* Allocate the catalog arrays: */ if(p->objncols>0 && p->numobjects>0) { errno=0; p->objcat=malloc(p->objncols*p->numobjects*sizeof *p->objcat); if(p->objcat==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->objcat in " "preprarearrays (ui.c)", p->objncols*p->numobjects*sizeof *p->objcat); } else p->objcat=NULL; if(p->clumpncols>0 && p->numclumps>0) { errno=0; p->clumpcat=malloc(p->clumpncols*p->numclumps * sizeof *p->clumpcat); if(p->clumpcat==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->clumpcat in " "preprarearrays (ui.c)", p->clumpncols*p->numclumps*sizeof *p->clumpcat); } else p->clumpcat=NULL; } /* Allocate two arrays to keep all the basic information about each object and clump. Note that there should be one row more than the total number of objects or clumps. This is because we want each label to be its row number and we don't have any object label of zero.*/ errno=0; p->oinfo=calloc(OCOLUMNS*(p->numobjects+1), sizeof *p->oinfo); if(p->oinfo==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->oinfo in mkcatalog " "(mkcatalog.c)", OCOLUMNS*(p->numobjects+1)*sizeof *p->oinfo); errno=0; p->cinfo=calloc(CCOLUMNS*(p->numclumps+1), sizeof *p->cinfo); if(p->cinfo==NULL) error(EXIT_FAILURE, errno, "%zu bytes for p->cinfo in mkcatalog " "(mkcatalog.c)", CCOLUMNS*(p->numclumps+1)*sizeof *p->cinfo); /* Set the shift values to NAN for all the objects and clumps: */ for(i=1;i<=p->numobjects;++i) p->oinfo[i*OCOLUMNS+OPOSSHIFTX]=p->oinfo[i*OCOLUMNS+OPOSSHIFTY]=NAN; for(i=1;i<=p->numclumps;++i) p->cinfo[i*CCOLUMNS+CPOSSHIFTX]=p->cinfo[i*CCOLUMNS+CPOSSHIFTY]=NAN; /* Allocate the random number generator: */ if(p->up.upperlimitmagset) { gsl_rng_env_setup(); if(p->envseed==0) gsl_rng_default_seed=gal_timing_time_based_rng_seed(); } /* Clean up: */ gal_linkedlist_free_sll(p->allcolsll); } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void setparams(int argc, char *argv[], struct mkcatalogparams *p) { struct gal_commonparams *cp=&p->cp; /* Set the non-zero initial values, the structure was initialized to have a zero value for all elements. */ cp->spack = SPACK; cp->verb = 1; cp->numthreads = num_processors(NPROC_CURRENT); cp->removedirinfo = 1; p->threshold = NAN; /* Read the arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Add the user default values and save them if asked. */ GAL_CONFIGFILES_CHECK_SET_CONFIG; /* Check if all the required parameters are set. */ checkifset(p); /* Do a sanity check. Note that if the user just wants to see the parameters and hasn't given any file name, sanity check is useless, because in MakeProfiles, sanitycheck just checks the file names. So we first have to check if an input */ if(p->up.inputname) sanitycheck(p); /* Make the array of input images. */ preparearrays(p); /* Print the values for each parameter. */ if(cp->printparams) GAL_CONFIGFILES_REPORT_PARAMETERS_SET; /* Everything is ready, notify the user of the program starting. */ if(cp->verb) { printf(SPACK_NAME" started on %s", ctime(&p->rawtime)); printf(" - Input %s (hdu: %s)\n", p->up.inputname, p->cp.hdu); if(p->up.masknameset) printf(" - Mask %s (hdu: %s)\n", p->up.maskname, p->up.mhdu); printf(" - Objects %s (hdu: %s)\n", p->up.objlabsname, p->up.objhdu); if(p->up.clumplabsname) printf(" - Clumps %s (hdu: %s)\n", p->up.clumplabsname, p->up.clumphdu); printf(" - Sky %s (hdu: %s)\n", p->up.skyname, p->up.skyhdu); printf(" - Sky STD %s (hdu: %s)\n", p->up.stdname, p->up.stdhdu); if(p->up.upperlimitmagset) { if(p->up.upmasknameset) printf(" - Upper limit mask: %s (hdu: %s)\n", p->up.inputname, p->cp.hdu); printf(" - RNG type for upper-limit magnitude: %s\n", gsl_rng_default->name); printf(" - RNG seed for upper-limit magnitude: %ld\n", gsl_rng_default_seed); } } } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void freeandreport(struct mkcatalogparams *p, struct timeval *t1) { /* Free all the allocated spaces: */ free(p->sky); free(p->std); free(p->objcat); free(p->cp.hdu); free(p->clumps); free(p->allcols); free(p->objects); free(p->objcols); free(p->clumpcat); free(p->ocatname); free(p->ccatname); free(p->clumpcols); free(p->up.objhdu); free(p->cp.output); free(p->up.skyhdu); free(p->up.stdhdu); free(p->up.clumphdu); if(p->upmask) free(p->upmask); if(p->up.mhduset) free(p->up.mhdu); if(p->wcs) wcsvfree(&p->nwcs, &p->wcs); if(p->up.skynameset) free(p->up.skyname); if(p->up.stdnameset) free(p->up.stdname); if(p->up.masknameset) free(p->up.maskname); if(p->up.objlabsnameset) free(p->up.objlabsname); if(p->up.clumplabsnameset) free(p->up.clumplabsname); /* Print the final message. */ if(p->cp.verb) gal_timing_report(t1, SPACK_NAME" finished in", 0); } gnuastro-0.2.33-8a3b/bin/mkcatalog/cite.h0000644000175000017500000000320412750745735014742 00000000000000/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CITE_H #define CITE_H #define MKCATALOGBIBTEX "" #define PRINTCITEABORT { \ printf("\nWe hope %s has been useful for your research.\n" \ "Citations are vital for the continued work on %s.\n" \ "Thank you for citing it in your research paper.\n" \ "\nPlease cite as \"%s\":\n\n%s\n\n%s", \ SPACK_NAME, SPACK_NAME, SPACK_STRING, \ GAL_STRINGS_MAIN_BIBTEX, MKCATALOGBIBTEX); \ exit(EXIT_SUCCESS); \ } #endif gnuastro-0.2.33-8a3b/bin/mkcatalog/main.h0000644000175000017500000004222712774157434014751 00000000000000/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include #include #include /* Progarm name macros: */ #define SPACK "astmkcatalog" /* Subpackage executable name. */ #define SPACK_NAME "MakeCatalog" /* Subpackage full name. */ #define SPACK_STRING SPACK_NAME" ("PACKAGE_NAME") "PACKAGE_VERSION /* Columns in the object and clump information tables ================================================== The information tables are not the final catalog, they keep all the necessary information to make the catalogs in a later step. The columns of that catalog can be specified by the user, while the information catalog colums are fixed. The basic idea is that through the first and second pass through the image, we fill in this information array. Then we build the catalog based on what the user has requested. FIRST ROW IS FLAG ROW: The object/clump IDs begin from one (1), not zero (0). So the first row in the oinfo, or cinfo arrays is not filled and we need to start from the second row (which as index 1). So we can use the first row as a flag for the appropriate columns. For example, the RA and Dec need to be calculated together, so once they are both calculated by RA (for example), there is no more need to calculate them again for Dec, or vice versa. So in this case, we set the first row of this column to 1 so if it is needed again, it is not recalculated. NOTE: The X and Y columns should be immediately after each other, this is necessary for converting to RA and Dec. NOTE: the total area and brightness of clumps in the objects can be found by using the clump information table in the end. According to the C standard, the first enum variable has a value of 0 (int), and when none are explicitly set (with an = sign), the values of the subsequent enum variables are 1 larger. We want column indexs that also start with zero, but setting the values by hand manually as preprocessor macros can be buggy (repeated numbers). So defining them as an enum is the perfect solution. Any future column that is to be added (or if any are removed), we (the developers) don't have to worry. */ enum objectcols { OAREA, /* Area of this object. */ OALLAREA, /* Object area irrespective of threshold. */ ONCLUMPS, /* Total number of clumps in this object. */ OBrightness, /* Sum of (flux-sky) in object. */ OFlxWhtX, /* Sum of (flux-sky)*x of this object. */ OFlxWhtY, /* Sum of (flux-sky)*y of this object. */ OFlxWhtXX, /* Sum of (flux-sky)*x*x of this object. */ OFlxWhtYY, /* Sum of (flux-sky)*y*y of this object. */ OFlxWhtXY, /* Sum of (flux-sky)*x*y of this object. */ OFlxWhtRA, /* RA of (OFlxWhtX, OFlxWhtY). */ OFlxWhtDec, /* Dec of (OFlxWhtX, OFlxWhtY). */ OAREAC, /* Area of clumps in this object. */ OBrightnessC, /* Brightness in object clumps. */ OUpperBright, /* Upper limit brightness for this object. */ OFlxWhtCX, /* Sum of (flux-sky)*x on object clumps. */ OFlxWhtCY, /* Sum of (flux-sky)*y on obj. clumps. */ OFlxWhtCXX, /* Sum of (flux-sky)*x*x on object clumps. */ OFlxWhtCYY, /* Sum of (flux-sky)*y*y on obj. clumps. */ OFlxWhtCXY, /* Sum of (flux-sky)*x*y on obj. clumps. */ OPOSSHIFTX, /* Shift in X to avoid rounding errors. */ OPOSSHIFTY, /* Shift in Y to avoid rounding errors. */ OFlxWhtCRA, /* RA of (OFlxWhtCX and OFlxWhtCY). */ OFlxWhtCDec, /* Dec of (OFlxWhtCX and OFlxWhtCY). */ OSKY, /* Sum of sky value on this object. */ OSTD, /* Sum of sky STD value on this object. */ OPosBright, /* Sum of positive image pixels for wht. */ OPosBrightC, /* Sum of positive image pixels for wht. */ OGeoX, /* Geometric center of object in X. */ OGeoY, /* Geometric center of object in Y. */ OGeoRA, /* RA of Geometric center of object. */ OGeoDec, /* Dec of Geometric center of object. */ OGeoXX, /* Second order geometric variable: X*X. */ OGeoYY, /* Second order geometric variable: Y*Y. */ OGeoXY, /* Second order geometric variable: X*Y. */ OGeoCX, /* Geometric center of clumps in object X. */ OGeoCY, /* Geometric center of clumps in object Y. */ OGeoCRA, /* Geometric center of clumps in obj. RA. */ OGeoCDec, /* Geometric center of clumps in obj. Dec. */ OGeoCXX, /* Second order geometric variable: X*X. */ OGeoCYY, /* Second order geometric variable: Y*Y. */ OGeoCXY, /* Second order geometric variable: X*Y. */ OCOLUMNS, /* Keep this last: total number of columns.*/ }; enum clumpcols { CHOSTOID, /* ID of object hosting this clump. */ CINHOSTID, /* ID of clump in host object. */ CAREA, /* Area of this clump. */ CALLAREA, /* Area of clump irrespective of threshold.*/ CFlxWhtX, /* Sum of flux*x of this clump. */ CFlxWhtY, /* Sum of flux*y of this clump. */ CFlxWhtXX, /* Sum of flux*x*x of this clump. */ CFlxWhtYY, /* Sum of flux*y*y of this clump. */ CFlxWhtXY, /* Sum of flux*x*y of this clump. */ CPOSSHIFTX, /* Shift in X to avoid rounding errors. */ CPOSSHIFTY, /* Shift in Y to avoid rounding errors. */ CFlxWhtRA, /* ra of (CFlxWhtX, CFlxWhtY). */ CFlxWhtDec, /* Dec of (CFlxWhtX, CFlxWhtY). */ CBrightness, /* River subtracted brightness. */ CNoRiverBrightness, /* Sky (not river) subtracted brightness. */ CUpperBright, /* Upper limit brightness for this clump. */ CRivAve, /* Average value in rivers around clump. */ CRivArea, /* Num river pixels around this clump. */ CSKY, /* Sum of sky value on this object. */ CSTD, /* Sum of sky STD value on this object. */ CPosBright, /* Sum of positive image pixels for wht. */ CGeoX, /* Geometric center of clump in X. */ CGeoY, /* Geometric center of clump in Y. */ CGeoRA, /* RA of Geometric center of clump. */ CGeoDec, /* Dec of Geometric center of clump. */ CGeoXX, /* Second order geometric moment. */ CGeoYY, /* Second order geometric moment. */ CGeoXY, /* Second order geometric moment. */ CCOLUMNS, /* Keep this last: total number of columns.*/ }; /* Codes for output columns ======================== The user can ask for any columns in any order, to enable that, we need a fixed number ID for each column. Again (similar to the argument for the information array columns), it is just important that these numbers be separate and defining them by hand can cause bugs. So we are defining them as enums here. */ enum outcols { CATID, CATHOSTOBJID, CATIDINHOSTOBJ, CATNUMCLUMPS, CATAREA, CATCLUMPSAREA, CATX, CATY, CATGEOX, CATGEOY, CATCLUMPSX, CATCLUMPSY, CATCLUMPSGEOX, CATCLUMPSGEOY, CATRA, CATDEC, CATGEORA, CATGEODEC, CATCLUMPSRA, CATCLUMPSDEC, CATCLUMPSGEORA, CATCLUMPSGEODEC, CATBRIGHTNESS, CATCLUMPSBRIGHTNESS, CATNORIVERBRIGHTNESS, CATMAGNITUDE, CATMAGNITUDEERR, CATCLUMPSMAGNITUDE, CATUPPERLIMITMAG, CATRIVERAVE, CATRIVERNUM, CATSN, CATSKY, CATSTD, CATSEMIMAJOR, CATSEMIMINOR, CATPOSITIONANGLE, CATGEOSEMIMAJOR, CATGEOSEMIMINOR, CATGEOPOSITIONANGLE, }; struct uiparams { char *inputname; /* Name of input file. */ char *maskname; /* Name of masked file. */ char *mhdu; /* HDU of mask image. */ char *objlabsname; /* Name of object labels file. */ char *objhdu; /* HDU of object labels image. */ char *clumplabsname; /* Name of clump labels file . */ char *clumphdu; /* HDU of clump labels image. */ char *skyname; /* Sky value image file name. */ char *skyhdu; /* Sky HDU name. */ char *stdname; /* Sky STD value image file name. */ char *stdhdu; /* Sky STD HDU name. */ char *upmaskname; /* Name of mask for upper magnitude. */ char *upmaskhdu; /* HDU Name of mask for upper mag. */ int masknameset; int mhduset; int objlabsnameset; int objhduset; int clumplabsnameset; int clumphduset; int skynameset; int skyhduset; int stdnameset; int stdhduset; int envseedset; int zeropointset; int skysubtractedset; int thresholdset; int intwidthset; int floatwidthset; int accuwidthset; int floatprecisionset; int accuprecisionset; int nsigmagset; int upmasknameset; int upmaskhduset; int upnumset; int upsclipmultipset; int upsclipaccuset; int upnsigmaset; int idset; int hostobjidset; int idinhostobjset; int numclumpsset; int areaset; int clumpsareaset; int xset; int yset; int geoxset; int geoyset; int clumpsxset; int clumpsyset; int clumpsgeoxset; int clumpsgeoyset; int raset; int decset; int georaset; int geodecset; int clumpsraset; int clumpsdecset; int clumpsgeoraset; int clumpsgeodecset; int brightnessset; int clumpsbrightnessset; int noriverbrightnessset; int magnitudeset; int magnitudeerrset; int clumpsmagnitudeset; int upperlimitmagset; int riveraveset; int rivernumset; int snset; int skyset; int stdset; int semimajorset; int semiminorset; int positionangleset; int geosemimajorset; int geosemiminorset; int geopositionangleset; }; struct mkcatalogparams { /* Other structures: */ struct uiparams up; /* User interface parameters. */ struct gal_commonparams cp; /* Common parameters. */ /* Input: */ float *img; /* Input image. */ long *objects; /* Object labels on each pixel. */ long *clumps; /* Clump labels on each pixel. */ float *sky; /* Sky value on each pixel. */ float *std; /* Sky STD value on each pixel. */ int nwcs; /* Number of WCS structures. */ struct wcsprm *wcs; /* Pointer to WCS structures. */ size_t s0; /* Size of input (first C axis). */ size_t s1; /* Size of input (second C axis). */ float zeropoint; /* Zeropoint magnitude of input. */ int skysubtracted; /* Input is already sky subtracted. */ double nsigmag; /* Multiple of Sky STD to report mag. */ double threshold; /* Only pixels larger than this *STD. */ int envseed; /* Use GSL_RNG_SEED for random seed. */ /* Output: */ char *ocatname; /* File name of object catalog. */ char *ccatname; /* File name of clump catalog. */ int intwidth; /* Width of integer columns. */ int floatwidth; /* Width of float columns. */ int accuwidth; /* Width of accurate float columns. */ int floatprecision; /* Floating point precision. */ int accuprecision; /* Accurate floating point precision. */ /* Upper limit: */ long *upmask; /* Mask array, only for upper liimit. */ size_t upnum; /* Number of random samples. */ float upsclipmultip; /* Sigma clip multiple for std calc. */ float upsclipaccu; /* Sigma clip accuracy for std calc. */ float upnsigma; /* Multiple of sigma for upper-limit. */ /* Operating mode: */ /* Internal: */ time_t rawtime; /* Starting time of the program. */ double *oinfo; /* Information for all the clumps. */ double *cinfo; /* Information for all the clumps. */ size_t numobjects; /* Total number of objects. */ size_t numclumps; /* Total number of clumps. */ struct gal_linkedlist_sll *allcolsll; /* All the input columns. */ size_t *allcols; /* Array keeping all the input cols. */ size_t allncols; /* Total number of input columns. */ size_t *objcols; /* Array of objcolsll. */ size_t *clumpcols; /* Array of clumpcolsll. */ size_t objncols; /* Num. columns in objects catalog. */ size_t clumpncols; /* Num. columns in clumps catalog. */ double *objcat; /* Output object catalog. */ double *clumpcat; /* Output clump catalog. */ size_t objcurcol; /* Current column in object catalog. */ size_t clumpcurcol; /* Current column in clump catalog. */ float minstd; /* For correction for counts/sec. */ float medstd; /* Median STD value (5 sigma mag). */ double cpscorr; /* Correction for counts/sec. */ double detsn; /* Detection S/N threshold. */ double clumpsn; /* Clumps S/N threshold. */ /* For going through the rows: */ size_t curcol; /* Current column in the catalog. */ size_t intcounter; /* Counter of the integer columns. */ size_t accucounter; /* Counter of the integer columns. */ int obj0clump1; /* Is this an object or clump catalog.*/ char *name; /* `Object' or `Clump'. */ double *cat; /* Either objcat or clumpcat. */ char *filename; /* Either ocatname or ccatname. */ size_t num; /* Either numobjects or numclumps. */ size_t numcols; /* Either objncols or clumpncols. */ double *info; /* Pointer to either oinfo or cinfo. */ size_t icols; /* Either OCOLUMNS or CCOLUMNS. */ char *unitp; /* Pointer to units array. */ size_t xshiftcol; /* Column to correct/shift positions. */ size_t yshiftcol; /* Column to correct/shift positions. */ char line[1500]; /* Comment line. */ char description[500]; /* The description of each row. */ int *intcols; /* Indexs of integer columns. */ int *accucols; /* Indexs of accurate columns. */ }; #endif gnuastro-0.2.33-8a3b/bin/mkcatalog/main.c0000644000175000017500000000324712774157327014744 00000000000000/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include /* Includes time.h and sys/time.h */ #include "main.h" #include "ui.h" /* needs main.h. */ #include "mkcatalog.h" /* needs main.h. */ int main (int argc, char *argv[]) { struct timeval t1; struct mkcatalogparams p={{0}, {0}, 0}; /* Set the starting time. */ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ setparams(argc, argv, &p); /* Run MakeProfiles */ mkcatalog(&p); /* Free all non-freed allocations. */ freeandreport(&p, &t1); /* Return successfully.*/ return EXIT_SUCCESS; } gnuastro-0.2.33-8a3b/bin/mkcatalog/Makefile.in0000644000175000017500000017317213004464627015715 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute 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GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ 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uninstall-am uninstall-binPROGRAMS uninstall-dist_sysconfDATA .PRECIOUS: Makefile # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: gnuastro-0.2.33-8a3b/bin/mkcatalog/astmkcatalog.conf0000644000175000017500000000275512774041352017166 00000000000000# Default parameters (System) for MakeCatalog. # MakeCatalog is part of GNU Astronomy Utitlies. # # Use the long option name of each paramter followed by # a value. The name and value should be separated by # atleast one of the following charaacters: # space, `,`, `=` or `:` # # Run with `--help` option or read the manual for a full # explanation of what each option means. # # NOTE I: All counting is from zero, not one. # NOTE II: Lines starting with `#` are ignored. # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Input: hdu 0 objhdu 1 clumphdu 2 skyhdu 3 stdhdu 4 zeropoint 0.0 skysubtracted 0 # Output: nsigmag 1 intwidth 6 floatwidth 13 accuwidth 15 floatprecision 3 accuprecision 8 # Upper limit magnitude: upnum 200 upsclipmultip 3 upsclipaccu 0.2 upnsigma 1 # Catalog columns: # sn 1 # std 1 # sky 1 # rivernum 1 # riverave 1 # clumpsdec 1 # clumpsra 1 # clumpsy 1 # clumpsx 1 # clumpsmagnitude 1 # clumpsarea 1 # numclumps 1 # magnitude 1 # area 1 # dec 1 # ra 1 # y 1 # x 1 # idinhostobj 1 # hostobjid 1 id 1 gnuastro-0.2.33-8a3b/bin/mkcatalog/Makefile.am0000644000175000017500000000301012773471525015672 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. NOTE: $(top_srcdir)/bootstrapped/lib is only necessary ## for internally compiled utilities and libraries. It must not be included ## during the tests since the bootstrapped libraries are not installed. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Utility and its sources bin_PROGRAMS = astmkcatalog astmkcatalog_SOURCES = main.c main.h cite.h ui.c ui.h args.h \ mkcatalog.c mkcatalog.h columns.c columns.h upperlimit.c upperlimit.h astmkcatalog_LDADD = $(top_builddir)/bootstrapped/lib/libgnu.la \ -lgnuastro ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astmkcatalog.conf gnuastro-0.2.33-8a3b/bin/imgwarp/0000755000175000017500000000000013004464724013417 500000000000000gnuastro-0.2.33-8a3b/bin/imgwarp/imgwarp.h0000644000175000017500000000301113001632537015145 00000000000000/********************************************************************* ImageWarp - Warp images using projective mapping. ImageWarp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef IMGTRANSFORM_H #define IMGTRANSFORM_H #include /* Limits to account for floating point errors: */ #define ABSOLUTEFLTERROR 1e-10 #define RELATIVEFLTERROR 1e-6 /* Internal structure. */ struct iwpparams { /* General input parameters: */ struct imgwarpparams *p; /* Thread parameters. */ size_t *indexs; /* Indexs to be used in this thread. */ pthread_barrier_t *b; /* Barrier to keep threads waiting. */ }; /* Extenal functions. */ void imgwarp(struct imgwarpparams *p); #endif gnuastro-0.2.33-8a3b/bin/imgwarp/imgwarp.c0000644000175000017500000004605013001632537015152 00000000000000/********************************************************************* ImageWarp - Warp images using projective mapping. ImageWarp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include "main.h" #include "imgwarp.h" /***************************************************************/ /************** MACROS ******************/ /***************************************************************/ /* Multiply a 2 element vector with a transformation matrix and put the result in the 2 element output array. It is assumed that the input is from a flat coordinate systemy. */ #define mappoint(V, T, O) \ { \ (O)[0]=( ( (T)[0]*(V)[0] + (T)[1]*(V)[1] + (T)[2] ) \ / ( (T)[6]*(V)[0] + (T)[7]*(V)[1] + (T)[8] ) ); \ (O)[1]=( ( (T)[3]*(V)[0] + (T)[4]*(V)[1] + (T)[5] ) \ / ( (T)[6]*(V)[0] + (T)[7]*(V)[1] + (T)[8] ) ); \ } \ /* A pixel's center is an integer value. This function will give the integer value that is nearest to a floating point number. Works for both positive and negative values and includes floating point errors. nearestint_halfhigher(0.5f) --> 1.0f */ #define nearestint_halfhigher(D) \ (ceil((D)) - (D) > 0.5f \ + GAL_POLYGON_ROUND_ERR ? ceil((D))-1.0f : ceil((D))) /* Similar to `nearestint_halflower' but: nearestint_halflower(0.5f) --> 0.0f; */ #define nearestint_halflower(D) \ (ceil((D)) - (D) > 0.5f - GAL_POLYGON_ROUND_ERR ? ceil((D))-1.0f : ceil((D))) #define ceilwitherr(D) \ ( fabs( nearbyint((D)) - (D) ) < GAL_POLYGON_ROUND_ERR \ ? nearbyint((D)) : nearbyint((D))+1 ) /***************************************************************/ /************** Processing function ******************/ /***************************************************************/ void * imgwarponthread(void *inparam) { struct iwpparams *iwp=(struct iwpparams*)inparam; struct imgwarpparams *p=iwp->p; long is0=p->is0, is1=p->is1; double area, nanarea, *input=p->input, v=NAN; size_t *extinds=p->extinds, *ordinds=p->ordinds; size_t i, j, ind, os1=p->onaxes[0], numcrn, numinput; double ocrn[8], icrn_base[8], icrn[8], *output=p->output; long x, y, xstart, xend, ystart, yend; /* Might be negative */ double pcrn[8], *outfpixval=p->outfpixval, ccrn[GAL_POLYGON_MAX_CORNERS]; for(i=0;(ind=iwp->indexs[i])!=GAL_THREADS_NON_THRD_INDEX;++i) { /* Initialize the output pixel value: */ numinput=0; output[ind]=nanarea=0.0f; /* Set the corners of this output pixel. The ind/os1 and ind%os1 start from 0. Note that the outfpixval already contains the correction for the fact that the FITS standard considers the center of first pixel to be at (1.0f, 1.0f).*/ ocrn[0]=(double)(ind%os1)-0.5f+outfpixval[0]; ocrn[1]=(double)(ind/os1)-0.5f+outfpixval[1]; ocrn[2]=(double)(ind%os1)+0.5f+outfpixval[0]; ocrn[3]=(double)(ind/os1)-0.5f+outfpixval[1]; ocrn[4]=(double)(ind%os1)-0.5f+outfpixval[0]; ocrn[5]=(double)(ind/os1)+0.5f+outfpixval[1]; ocrn[6]=(double)(ind%os1)+0.5f+outfpixval[0]; ocrn[7]=(double)(ind/os1)+0.5f+outfpixval[1]; /* Transform the four corners of the output pixel to the input image coordinates. */ for(j=0;j<4;++j) mappoint(&ocrn[j*2], p->inverse, &icrn_base[j*2]); /* Using the known relationships between the vertice locations, put everything in the right place: */ xstart = nearestint_halfhigher( icrn_base[extinds[0]] ); xend = nearestint_halflower( icrn_base[extinds[1]] ) + 1; ystart = nearestint_halfhigher( icrn_base[extinds[2]] ); yend = nearestint_halflower( icrn_base[extinds[3]] ) + 1; icrn[0]=icrn_base[ordinds[0]*2]; icrn[1]=icrn_base[ordinds[0]*2+1]; icrn[2]=icrn_base[ordinds[1]*2]; icrn[3]=icrn_base[ordinds[1]*2+1]; icrn[4]=icrn_base[ordinds[2]*2]; icrn[5]=icrn_base[ordinds[2]*2+1]; icrn[6]=icrn_base[ordinds[3]*2]; icrn[7]=icrn_base[ordinds[3]*2+1]; /* For a check: if(ind==9999) { printf("\n\n\nind: %zu: (%zu, %zu):\n", ind, ind%os1+1, ind/os1+1); for(j=0;j<4;++j) printf("(%.3f, %.3f) --> (%.3f, %.3f)\n", ocrn[j*2], ocrn[j*2+1], icrn_base[j*2], icrn_base[j*2+1]); printf("------- Ordered -------\n"); for(j=0;j<4;++j) printf("(%.3f, %.3f)\n", icrn[j*2], icrn[j*2+1]); printf("------- Start and ending pixels -------\n"); printf("X: %ld -- %ld\n", xstart, xend); printf("Y: %ld -- %ld\n", ystart, yend); } */ /* Go over all the input pixels that are covered. Note that x and y are the centers of the pixel. */ for(y=ystart;yis0 ) continue; pcrn[1]=y-0.5f; pcrn[3]=y-0.5f; pcrn[5]=y+0.5f; pcrn[7]=y+0.5f; for(x=xstart;xis1 ) continue; /* Read the value of the input pixel. */ v=input[(y-1)*is1+x-1]; pcrn[0]=x-0.5f; pcrn[2]=x+0.5f; pcrn[4]=x+0.5f; pcrn[6]=x-0.5f; /* Find the overlapping (clipped) polygon: */ gal_polygon_clip(icrn, 4, pcrn, 4, ccrn, &numcrn); area=gal_polygon_area(ccrn, numcrn); /* Add the fractional value of this pixel. If this output pixel covers a NaN pixel in the input grid, then calculate the area of this NaN pixel to account for it later. */ if( isnan(v) ) nanarea+=area; else { ++numinput; output[ind]+=v*area; } /* For a polygon check: if(ind==9999) { printf("%zu -- (%zd, %zd):\n", ind, x, y); printf("icrn:\n"); for(j=0;j<4;++j) printf("\t%.3f, %.3f\n", icrn[j*2], icrn[j*2+1]); printf("pcrn:\n"); for(j=0;j<4;++j) printf("\t%.3f, %.3f\n", pcrn[j*2], pcrn[j*2+1]); printf("ccrn:\n"); for(j=0;j (%zu) %f\n", v*gal_polygon_area(ccrn, numcrn), numinput, output[ind]); */ } } /* Correct for the area covered by a NaN. The basic idea is this: The full pixel (with area `A') would have a value of `F'. But we have only measured the value `f' over the area `a', so a simple linear extrapolation would give: F=fA/a. */ if(numinput && nanarea!=0.0f) { /* For a check: printf("%zu: %f/%f --> %f\n", ind, nanarea, p->opixarea, nanarea/p->opixarea); */ if(nanarea/p->opixareamaxblankfrac) output[ind]*=p->opixarea/(p->opixarea-nanarea); else numinput=0; } /* Write the final value to disk: */ if(numinput==0 && p->zerofornoinput==0) { output[ind]=NAN; ++p->numnul; } } /* Wait until all other threads finish. */ if(p->cp.numthreads>1) pthread_barrier_wait(iwp->b); return NULL; } /***************************************************************/ /************** Preparations ******************/ /***************************************************************/ /* Do all the preparations. Make the output array. We transform the four corners of the image into the output space. To find the four sides of the image. About fpixel and lpixel. The point is that we don't want to spend time, transforming any pixels which we know will not be in the input image. Find the proper order of transformed pixel corners from the output array to the input array. The order is fixed for all the pixels in the image altough the scale might change. */ void imgwarppreparations(struct imgwarpparams *p) { double output[8], forarea[8]; double icrn[8]={0,0,0,0,0,0,0,0}; size_t i, *extinds=p->extinds, size; double xmin=DBL_MAX, xmax=-DBL_MAX, ymin=DBL_MAX, ymax=-DBL_MAX; double ocrn[8]={0.5f,0.5f, 1.5f,0.5f, 0.5f,1.5f, 1.5f, 1.5f}; double input[8]={0.5f,0.5f, p->is1+0.5f, 0.5f, 0.5f, p->is0+0.5f, p->is1+0.5f, p->is0+0.5f}; /* Find the range of pixels of the input image. All the input positions are moved to the negative by half a pixel since the center of the pixel is an integer value.*/ for(i=0;i<4;++i) { mappoint(&input[i*2], p->matrix, &output[i*2]); if(output[i*2]xmax) xmax = output[i*2]; if(output[i*2+1]ymax) ymax = output[i*2+1]; } /* For a check: for(i=0;i<4;++i) printf("(%.3f, %.3f) --> (%.3f, %.3f)\n", input[i*2], input[i*2+1], output[i*2], output[i*2+1]); printf("xmin: %.3f\nxmax: %.3f\nymin: %.3f\nymax: %.3f\n", xmin, xmax, ymin, ymax); */ /* Set the final size of the image. The X axis is horizontal. The reason we are using the halflower variation of `nearestint' for the maximums is that these points are the farthest extremes of the input image. If they are half a pixel value, they should point to the pixel before. */ p->onaxes[0]=nearestint_halflower(xmax)-nearestint_halfhigher(xmin)+1; p->onaxes[1]=nearestint_halflower(ymax)-nearestint_halfhigher(ymin)+1; p->outfpixval[0]=nearestint_halfhigher(xmin); p->outfpixval[1]=nearestint_halfhigher(ymin); /* For a check: printf("Wrapped:\n"); printf("onaxes: (%zu, %zu)\n", p->onaxes[0], p->onaxes[1]); printf("outfpixval=(%.4f, %.4f)\n", p->outfpixval[0], p->outfpixval[1]); */ /* We now know the size of the output and the starting and ending coordinates in the output image (bottom left corners of pixels) for the transformation. */ errno=0; size=p->onaxes[0]*p->onaxes[1]; p->output=malloc(size*sizeof *p->output); if(p->output==NULL) error(EXIT_FAILURE, errno, "%zu bytes for the output array", size*sizeof *p->output); /* Order the corners of the inverse-transformed pixel (from the output to the input) in an anti-clockwise transformation. In a general homographic transform, the scales of the output pixels may change, but the relative positions of the corners will not. */ for(i=0;i<4;++i) { ocrn[i*2] += p->outfpixval[0]; ocrn[i*2+1] += p->outfpixval[1]; mappoint(&ocrn[i*2], p->inverse, &icrn[i*2]); } /* Order the transformed output pixel. */ gal_polygon_ordered_corners(icrn, 4, p->ordinds); /* Find the area of the output pixel in units of the input pixel, this is necessary if we are going to have NAN pixels in the image to account for the area lost due to a NAN value. */ for(i=0;i<4;++i) { forarea[2*i]=icrn[2*p->ordinds[i]]; forarea[2*i+1]=icrn[2*p->ordinds[i]+1]; } p->opixarea=gal_polygon_area(forarea, 4); /* Find which index after transformation will have the minimum and maximum positions along the two axises. We can't use the starting loop because that is based on the input image which can be not-a-square! So we do it here where pixels are squares. */ xmin=DBL_MAX; xmax=-DBL_MAX; ymin=DBL_MAX; ymax=-DBL_MAX; for(i=0;i<4;++i) { if(icrn[i*2]xmax) { xmax=icrn[i*2]; extinds[1]=i*2; } if(icrn[i*2+1]ymax) { ymax=icrn[i*2+1]; extinds[3]=i*2+1; } } /* For a check: for(i=0;i<4;++i) printf("(%.3f, %.3f) --> (%.3f, %.3f)\n", ocrn[i*2], ocrn[i*2+1], icrn[i*2], icrn[i*2+1]); printf("xmin: %.3f\nxmax: %.3f\nymin: %.3f\nymax: %.3f\n", xmin, xmax, ymin, ymax); */ } /* Correct the WCS coordinates (Multiply the 2x2 PC matrix of the WCS structure by the INVERSE of the transform in 2x2 form that has been converted from homogeneous coordinates). Then Multiply the crpix array with the ACTUAL transformation matrix. */ void correctwcssaveoutput(struct imgwarpparams *p) { size_t i; void *array; char keyword[9*FLEN_KEYWORD]; double *m=p->matrix, diff, dx, dy; struct gal_fits_key_ll *headers=NULL; double tpc[4], tcrpix[3], *crpix=p->wcs->crpix, *pc=p->wcs->pc; double tinv[4]={p->inverse[0]/p->inverse[8], p->inverse[1]/p->inverse[8], p->inverse[3]/p->inverse[8], p->inverse[4]/p->inverse[8]}; if(p->correctwcs && p->wcs) { /* Correct the PC matrix: */ tpc[0]=pc[0]*tinv[0]+pc[1]*tinv[2]; tpc[1]=pc[0]*tinv[1]+pc[1]*tinv[3]; tpc[2]=pc[2]*tinv[0]+pc[3]*tinv[2]; tpc[3]=pc[2]*tinv[1]+pc[3]*tinv[3]; pc[0]=tpc[0]; pc[1]=tpc[1]; pc[2]=tpc[2]; pc[3]=tpc[3]; /* Correct the CRPIX point. The +1 in the end of the last two lines is because FITS counts from 1. */ tcrpix[0]=m[0]*crpix[0]+m[1]*crpix[1]+m[2]; tcrpix[1]=m[3]*crpix[0]+m[4]*crpix[1]+m[5]; tcrpix[2]=m[6]*crpix[0]+m[7]*crpix[1]+m[8]; crpix[0]=tcrpix[0]/tcrpix[2]-p->outfpixval[0]+1; crpix[1]=tcrpix[1]/tcrpix[2]-p->outfpixval[1]+1; } /* Convert the output to the input image format: */ if(p->inputbitpix==DOUBLE_IMG || p->doubletype) { array=p->output; p->inputbitpix=DOUBLE_IMG; /* Not converted and p->doubletype==1 */ } else gal_fits_change_type((void **)p->output, DOUBLE_IMG, p->onaxes[1]*p->onaxes[0], p->numnul, &array, p->inputbitpix); /* Add the appropriate headers: */ gal_fits_file_name_in_keywords("INF", p->up.inputname, &headers); for(i=0;i<9;++i) { sprintf(&keyword[i*FLEN_KEYWORD], "WMTX%zu_%zu", i/3+1, i%3+1); gal_fits_add_to_key_ll_end(&headers, TDOUBLE, &keyword[i*FLEN_KEYWORD], 0, &p->matrix[i], 0, "Warp matrix " "element value.", 0, NULL); } /* Due to floating point errors extremely small values of PC matrix can be set to zero and extremely small differences between PC1_1 and PC2_2 can be ignored. The reason for all the `fabs' functions is because the signs are usually different.*/ if( p->wcs->pc[1]wcs->pc[1]=0.0f; if( p->wcs->pc[2]wcs->pc[2]=0.0f; gal_wcs_pixel_scale_deg(p->wcs, &dx, &dy); diff=fabs(p->wcs->pc[0])-fabs(p->wcs->pc[3]); if( fabs(diff/dx)wcs->pc[3] = ( (p->wcs->pc[3] < 0.0f ? -1.0f : 1.0f) * fabs(p->wcs->pc[0]) ); /* Save the output: */ gal_fits_array_to_file(p->cp.output, "Warped", p->inputbitpix, array, p->onaxes[1], p->onaxes[0], p->numnul, p->wcs, headers, SPACK_STRING); if(array!=p->output) free(array); } /***************************************************************/ /************** Outside function ******************/ /***************************************************************/ void imgwarp(struct imgwarpparams *p) { int err; pthread_t t; /* All thread ids saved in this, not used. */ pthread_attr_t attr; pthread_barrier_t b; struct iwpparams *iwp; size_t i, nb, *indexs, thrdcols; size_t nt=p->cp.numthreads, size; /* Set the number of output blank pixels to zero: */ p->numnul=0; /* Array keeping thread parameters for each thread. */ errno=0; iwp=malloc(nt*sizeof *iwp); if(iwp==NULL) error(EXIT_FAILURE, errno, "%zu bytes in imgwarp " "(imgwarp.c) for iwp", nt*sizeof *iwp); /* Prepare the output array and all the necessary things: */ imgwarppreparations(p); /* Distribute the output pixels into the threads: */ size=p->onaxes[0]*p->onaxes[1]; gal_threads_dist_in_threads(size, nt, &indexs, &thrdcols); /* Start the convolution. */ if(nt==1) { iwp[0].p=p; iwp[0].indexs=indexs; imgwarponthread(&iwp[0]); } else { /* Initialize the attributes. Note that this running thread (that spinns off the nt threads) is also a thread, so the number the barrier should be one more than the number of threads spinned off. */ if(sizeoutput); } gnuastro-0.2.33-8a3b/bin/imgwarp/args.h0000644000175000017500000002000413002504751014431 00000000000000/********************************************************************* ImageWarp - Warp images using projective mapping. ImageWarp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef ARGS_H #define ARGS_H #include #include #include /**************************************************************/ /************** argp.h definitions ***************/ /**************************************************************/ /* Definition parameters for the argp: */ const char *argp_program_version=SPACK_STRING"\n"GAL_STRINGS_COPYRIGHT "\n\nWritten by Mohammad Akhlaghi"; const char *argp_program_bug_address=PACKAGE_BUGREPORT; static char args_doc[] = "[matrix.txt] ASTRdata ..."; const char doc[] = /* Before the list of options: */ GAL_STRINGS_TOP_HELP_INFO SPACK_NAME" will warp/transform the input image using an input coordinate " "matrix. Currently it accepts any general projective mapping (which " "includes affine mappings as a subset). \n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /* Available letters for short options: c g i j k l u v w x y A B C E F G H I J L M O Q R T U W X Y Z Number keys used: <=503 Options with keys (second structure element) larger than 500 do not have a short version. */ static struct argp_option options[] = { { 0, 0, 0, 0, "Input:", 1 }, { "matrix", 'm', "STR", 0, "Warp/Transform matrix elements.", 1 }, { "hstartwcs", 501, "INT", 0, "Header keyword number to start reading WCS.", 1 }, { "hendwcs", 502, "INT", 0, "Header keyword number to stop reading WCS.", 1 }, { "nofitscorrect", 503, 0, 0, "Do not shift to correct for FITS positioning.", 1 }, { 0, 0, 0, 0, "Output:", 2 }, { "nowcscorrection", 'n', 0, 0, "Do not correct input image WCS.", 2 }, { "zerofornoinput", 'z', 0, 0, "Set pixels with no input to zero not blank.", 2 }, { "doubletype", 'd', 0, 0, "Do not convert output to input image type.", 2 }, { "maxblankfrac", 'b', "FLT", 0, "Maximum fraction of area covered by blank.", 2 }, { 0, 0, 0, 0, "Modular warpings:", 3 }, { "align", 'a', 0, 0, "Align the image and celestial axes.", 3 }, { "rotate", 'r', "FLT", 0, "Rotate by the given angle in degrees.", 3 }, { "scale", 's', "FLT[,FLT]", 0, "Scale along the given axis(es).", 3 }, { "flip", 'f', "FLT[,FLT]", 0, "Flip along the given axis(es).", 3 }, { "shear", 'e', "FLT[,FLT]", 0, "Shear along the given axis(es).", 3 }, { "translate", 't', "FLT[,FLT]", 0, "Translate along the given axis(es).", 3 }, { "project", 'p', "FLT[,FLT]", 0, "Project along the given axis(es).", 3 }, { 0, 0, 0, 0, "Operating modes:", -1 }, {0} }; /* Parse a single option: */ static error_t parse_opt(int key, char *arg, struct argp_state *state) { /* Save the arguments structure: */ struct imgwarpparams *p = state->input; /* Set the pointer to the common parameters for all programs here: */ state->child_inputs[0]=&p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); switch(key) { /* Input: */ case 'm': p->up.matrixstring=arg; p->up.matrixstringset=1; break; case 501: gal_checkset_sizet_el_zero(arg, &p->hstartwcs, "hstartwcs", key, SPACK, NULL, 0); p->up.hstartwcsset=1; break; case 502: gal_checkset_sizet_el_zero(arg, &p->hendwcs, "hendwcs", key, SPACK, NULL, 0); p->up.hendwcsset=1; break; /* Output: */ case 'n': p->correctwcs=0; break; case 'z': p->zerofornoinput=1; break; case 'd': p->doubletype=1; break; case 'b': gal_checkset_float_l_0_s_1(arg, &p->maxblankfrac, "maxblankfrac", key, SPACK, NULL, 0); p->up.maxblankfracset=1; break; case 503: p->up.nofitscorrect=1; p->up.nofitscorrectset=1; break; /* Modular warpings */ case 'a': add_to_optionwapsll(&p->up.owll, ALIGN_WARP, NULL); break; case 'r': add_to_optionwapsll(&p->up.owll, ROTATE_WARP, arg); break; case 's': add_to_optionwapsll(&p->up.owll, SCALE_WARP, arg); break; case 'f': add_to_optionwapsll(&p->up.owll, FLIP_WARP, arg); break; case 'e': add_to_optionwapsll(&p->up.owll, SHEAR_WARP, arg); break; case 't': add_to_optionwapsll(&p->up.owll, TRANSLATE_WARP, arg); break; case 'p': add_to_optionwapsll(&p->up.owll, PROJECT_WARP, arg); break; /* Read the non-option arguments: */ case ARGP_KEY_ARG: /* See what type of input value it is and put it in. */ if( gal_fits_name_is_fits(arg) ) { if(p->up.inputname) argp_error(state, "only one input image should be given"); else p->up.inputname=arg; } else { if(p->up.matrixname) argp_error(state, "only one warp/transformation matrix " "should be given"); else p->up.matrixname=arg; } break; /* The command line options and arguments are finished. */ case ARGP_KEY_END: if(p->cp.setdirconf==0 && p->cp.setusrconf==0 && p->cp.printparams==0) { if(state->arg_num==0) argp_error(state, "no argument given"); if(p->up.inputname==NULL) argp_error(state, "no input FITS image(s) provided"); } break; default: return ARGP_ERR_UNKNOWN; } return 0; } /* Specify the children parsers: */ struct argp_child children[]= { {&commonargp, 0, NULL, 0}, {0, 0, 0, 0} }; /* Basic structure defining the whole argument reading process. */ static struct argp thisargp = {options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif gnuastro-0.2.33-8a3b/bin/imgwarp/ui.h0000644000175000017500000000276113002504750014123 00000000000000/********************************************************************* ImageWarp - Warp images using projective mapping. ImageWarp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef UI_H #define UI_H /* Macros for various types of standard transformation.*/ enum standard_warps { ALIGN_WARP, ROTATE_WARP, SCALE_WARP, FLIP_WARP, SHEAR_WARP, TRANSLATE_WARP, PROJECT_WARP, }; /* Functions */ void add_to_optionwapsll(struct optionwarpsll **list, int type, char *value); void parse_two_values(char *str, double *v1, double *v2); void setparams(int argc, char *argv[], struct imgwarpparams *p); void freeandreport(struct imgwarpparams *p, struct timeval *t1); #endif gnuastro-0.2.33-8a3b/bin/imgwarp/ui.c0000644000175000017500000007466713002706671014142 00000000000000/********************************************************************* ImageWarp - Warp images using projective mapping. ImageWarp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* From Gnulib. */ #include #include #include #include /* Includes time.h and sys/time.h */ #include #include #include #include "main.h" #include "ui.h" /* Needs main.h */ #include "args.h" /* Needs main.h, includes argp.h. */ /* Set the file names of the places where the default parameters are put. */ #define CONFIG_FILE SPACK CONF_POSTFIX #define SYSCONFIG_FILE SYSCONFIG_DIR "/" CONFIG_FILE #define USERCONFIG_FILEEND USERCONFIG_DIR CONFIG_FILE #define CURDIRCONFIG_FILE CURDIRCONFIG_DIR CONFIG_FILE /**************************************************************/ /************** Options and parameters ***************/ /**************************************************************/ void readconfig(char *filename, struct imgwarpparams *p) { FILE *fp; size_t lineno=0, len=200; char *line, *name, *value; struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; char key='a'; /* Not used, just a place holder. */ /* When the file doesn't exist or can't be opened, it is ignored. It might be intentional, so there is no error. If a parameter is missing, it will be reported after all defaults are read. */ fp=fopen(filename, "r"); if (fp==NULL) return; /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); /* Read the tokens in the file: */ while(getline(&line, &len, fp) != -1) { /* Prepare the "name" and "value" strings, also set lineno. */ GAL_CONFIGFILES_START_READING_LINE; /* Inputs: */ if(strcmp(name, "hdu")==0) gal_checkset_allocate_copy_set(value, &cp->hdu, &cp->hduset); else if(strcmp(name, "hstartwcs")==0) { if(up->hstartwcsset) continue; gal_checkset_sizet_el_zero(value, &p->hstartwcs, name, key, SPACK, filename, lineno); up->hstartwcsset=1; } else if(strcmp(name, "hendwcs")==0) { if(up->hendwcsset) continue; gal_checkset_sizet_el_zero(value, &p->hendwcs, name, key, SPACK, filename, lineno); up->hendwcsset=1; } /* Outputs */ else if(strcmp(name, "matrix")==0) gal_checkset_allocate_copy_set(value, &up->matrixstring, &up->matrixstringset); else if(strcmp(name, "output")==0) gal_checkset_allocate_copy_set(value, &cp->output, &cp->outputset); else if(strcmp(name, "maxblankfrac")==0) { if(up->maxblankfracset) continue; gal_checkset_float_l_0_s_1(value, &p->maxblankfrac, name, key, SPACK, filename, lineno); up->maxblankfracset=1; } else if(strcmp(name, "nofitscorrect")==0) { if(up->nofitscorrectset) continue; gal_checkset_int_zero_or_one(value, &up->nofitscorrect, name, key, SPACK, filename, lineno); up->nofitscorrectset=1; } /* Modular warpings */ else if(strcmp(name, "align")==0) add_to_optionwapsll(&p->up.owll, ALIGN_WARP, NULL); else if(strcmp(name, "rotate")==0) add_to_optionwapsll(&p->up.owll, ROTATE_WARP, value); else if(strcmp(name, "scale")==0) add_to_optionwapsll(&p->up.owll, SCALE_WARP, value); else if(strcmp(name, "flip")==0) add_to_optionwapsll(&p->up.owll, FLIP_WARP, value); else if(strcmp(name, "shear")==0) add_to_optionwapsll(&p->up.owll, SHEAR_WARP, value); else if(strcmp(name, "translate")==0) add_to_optionwapsll(&p->up.owll, TRANSLATE_WARP, value); else if(strcmp(name, "project")==0) add_to_optionwapsll(&p->up.owll, PROJECT_WARP, value); /* Operating modes: */ /* Read options common to all programs */ GAL_CONFIGFILES_READ_COMMONOPTIONS_FROM_CONF else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s` not recognized.\n", name); } free(line); fclose(fp); } void printvalues(FILE *fp, struct imgwarpparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; /* Print all the options that are set. Separate each group with a commented line explaining the options in that group. */ fprintf(fp, "\n# Input image:\n"); if(cp->hduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("hdu", cp->hdu); if(up->hstartwcsset) fprintf(fp, CONF_SHOWFMT"%zu\n", "hstartwcs", p->hstartwcs); if(up->hendwcsset) fprintf(fp, CONF_SHOWFMT"%zu\n", "hendwcs", p->hendwcs); fprintf(fp, "\n# Output parameters:\n"); if(up->matrixstringset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("matrix", up->matrixstring); if(cp->outputset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("output", cp->output); if(up->maxblankfracset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "maxblankfrac", p->maxblankfrac); fprintf(fp, "\n# Modular transformations:\n"); if(up->nofitscorrectset) fprintf(fp, CONF_SHOWFMT"%d\n", "nofitscorrect", up->nofitscorrect); /* For the operating mode, first put the macro to print the common options, then the (possible options particular to this program). */ fprintf(fp, "\n# Operating mode:\n"); GAL_CONFIGFILES_PRINT_COMMONOPTIONS; } /* Note that numthreads will be used automatically based on the configure time. */ void checkifset(struct imgwarpparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; int intro=0; if(cp->hduset==0) GAL_CONFIGFILES_REPORT_NOTSET("hdu"); if(up->maxblankfracset==0) GAL_CONFIGFILES_REPORT_NOTSET("maxblankfrac"); GAL_CONFIGFILES_END_OF_NOTSET_REPORT; } /**************************************************************/ /********** Modular matrix linked list *************/ /**************************************************************/ void add_to_optionwapsll(struct optionwarpsll **list, int type, char *value) { double v1=NAN, v2=NAN; char *tailptr, *secondstr; struct optionwarpsll *newnode; /* Allocate the necessary space. */ errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "%zu bytes for newnode in " "add_to_optionwarpsll", sizeof *newnode); /* Read the numbers when necessary. */ if(value) { /* Parse the first number */ v1=strtod(value, &tailptr); if(tailptr==value) error(EXIT_FAILURE, 0, "The start of the string `%s' could not be " "read as a number", value); /* If there is any white space characters, ignore them and make sure that the first character is a coma (`,'). */ secondstr=tailptr; while(isspace(*secondstr)) ++secondstr; if(*secondstr==',') { /* If the type is rotate, then print an error since rotate only needs one input, not two. */ if(type==ROTATE_WARP) error(EXIT_FAILURE, 0, "The `--rotate' (`-r') option only needs " "one input number, not more. It was given `%s'", value); /* Ignore the coma. */ ++secondstr; /* Read the second number: */ v2=strtod(secondstr, &tailptr); if(tailptr==secondstr) error(EXIT_FAILURE, 0, "The second part (after the coma) of " "`%s' (`%s') could not be read as a number", value, secondstr); } /* If there was only one number given, secondstr will be '\0' when control reaches here. */ else if(*secondstr!='\0') error(EXIT_FAILURE, 0, "the character between the two numbers (`%s') " "must be a coma (`,')\n", value); } /* Put in the values. Note that both v1 and v2 were initialized to NaN, so if v2 is not given, it will be NaN and the later function can decide what it wants to replace it with.*/ newnode->v1=v1; newnode->v2=v2; newnode->type=type; newnode->next=*list; /* Set list to point to the new node. */ *list=newnode; } /* Allocate space for a new node: */ struct optionwarpsll * alloc_owll_node(void) { struct optionwarpsll *newnode; errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "%zu bytes for newnode in " "add_to_optionwarpsll", sizeof *newnode); return newnode; } /* The input list of warpings are recorded in a last-in-first-out order. So we reverse the order and also add the transformations necessary for the FITS definition (where the center of the pixel has a value of 1, not its corner. */ void prepare_optionwapsll(struct imgwarpparams *p) { struct optionwarpsll *tmp, *next, *newnode, *prepared=NULL; /* Add the FITS correction for the first warp (before everything else). IMPORTANT: This is the last transform that will be done, so we have to translate the image by -0.5.*/ if(!p->up.nofitscorrect) { newnode = alloc_owll_node(); newnode->v1 = newnode->v2 = -0.5f; newnode->type = TRANSLATE_WARP; newnode->next = prepared; prepared = newnode; } /* Put in the rest of the warpings */ tmp=p->up.owll; while(tmp!=NULL) { /* Allocate space for the new element, and put the values in. */ newnode = alloc_owll_node(); newnode->v1 = tmp->v1; newnode->v2 = tmp->v2; newnode->type = tmp->type; newnode->next = prepared; /* Now that previous nodes have been linked to next, set the reversed to the new node. */ prepared = newnode; /* Now keep the next element and free the old allocated space. */ next = tmp->next; free(tmp); tmp = next; } /* Add the FITS correction for the last warp (after everything else). IMPORTANT: This is the first transform that will be done, so we have to translate the image by +0.5.*/ if(!p->up.nofitscorrect) { newnode = alloc_owll_node(); newnode->v1 = newnode->v2 = 0.5f; newnode->type = TRANSLATE_WARP; newnode->next = prepared; prepared = newnode; } /* Put the pointer in the output */ p->up.owll=prepared; } /**************************************************************/ /************* Fill temporary matrix *****************/ /**************************************************************/ void read_matrix(struct imgwarpparams *p) { char *t, *tailptr; size_t i, counter=0, m0, m1; double *matrix=p->matrix, rmatrix[9], *fmatrix; /* Read the matrix either as a file or from the command-line. */ if(p->up.matrixname) { gal_txtarray_txt_to_array(p->up.matrixname, &fmatrix, &m0, &m1); counter=m0*m1; for(i=0;i<(counter<9 ? counter : 9);++i) rmatrix[i]=fmatrix[i]; free(fmatrix); } else { t=p->up.matrixstring; while(*t!='\0') { switch(*t) { case ' ': case '\t': case ',': ++t; break; default: errno=0; rmatrix[counter++]=strtod(t, &tailptr); if(errno) error(EXIT_FAILURE, errno, "reading `%s`", t); if(tailptr==t) error(EXIT_FAILURE, 0, "the provided string `%s' for " "matrix could not be read as a number", t); t=tailptr; if(counter>9) /* Note that it was incremented! */ error(EXIT_FAILURE, 0, "there are %zu elements in `%s', " "there should be 4 or 9", counter, p->up.matrixstring); /*printf("%f, %s\n", p->matrix[counter-1], t);*/ } } } /* If there was 4 elements (a 2 by 2 matrix), put them into a 3 by 3 matrix. */ if(counter==4) { /* Fill in the easy 3 by 3 matrix: */ matrix[0]=rmatrix[0]; matrix[1]=rmatrix[1]; matrix[3]=rmatrix[2]; matrix[4]=rmatrix[3]; matrix[6]=0.0f; matrix[7]=0.0f; matrix[8]=1.0f; /* If we need to correct for the FITS standard, then correc the last two elements. Recall that the coordinates of the center of the first pixel in the FITS standard are 1. We want 0 to be the coordinates of the bottom corner of the image. 1 0 0.5 a b 0 a b 0.5 0 1 0.5 * c d 0 = c d 0.5 0 0 1 0 0 1 0 0 1 and a b 0.5 1 0 -0.5 a b (a*-0.5)+(b*-0.5)+0.5 c d 0.5 * 0 1 -0.5 = c d (c*-0.5)+(d*-0.5)+0.5 0 0 1 0 0 1 0 0 1 */ if(p->up.nofitscorrect) matrix[2] = matrix[5] = 0.0f; else { matrix[2] = ((rmatrix[0] + rmatrix[1]) * -0.5f) + 0.5f; matrix[5] = ((rmatrix[2] + rmatrix[3]) * -0.5f) + 0.5f; } } else if (counter==9) { matrix[0]=rmatrix[0]; matrix[1]=rmatrix[1]; matrix[2]=rmatrix[2]; matrix[3]=rmatrix[3]; matrix[4]=rmatrix[4]; matrix[5]=rmatrix[5]; matrix[6]=rmatrix[6]; matrix[7]=rmatrix[7]; matrix[8]=rmatrix[8]; } else error(EXIT_FAILURE, 0, "there are %zu numbers in the string `%s'! " "It should contain 4 or 9 numbers (for a 2 by 2 or 3 by 3 " "matrix)", counter, p->up.matrixstring); } /* Set the matrix so the image is aligned with the axises. Note that WCSLIB automatically fills the CRPI */ void makealignmatrix(struct imgwarpparams *p, double *tmatrix) { double A, dx, dy; double amatrix[4]; double w[4]={0,0,0,0}; /* Check if there is only two WCS axises: */ if(p->wcs->naxis!=2) error(EXIT_FAILURE, 0, "the WCS structure of %s (hdu: %s) has %d " "axises. For the `--align' option to operate it must be 2", p->up.inputname, p->cp.hdu, p->wcs->naxis); /* Depending on the type of data, make the input matrix. Note that wcs->altlin is actually bit flags, not integers, so we have to compare with powers of two. */ if(p->wcs->altlin |= 1) { w[0]=p->wcs->cdelt[0]*p->wcs->pc[0]; w[1]=p->wcs->cdelt[0]*p->wcs->pc[1]; w[2]=p->wcs->cdelt[1]*p->wcs->pc[2]; w[3]=p->wcs->cdelt[1]*p->wcs->pc[3]; } if(p->wcs->altlin |= 2) { w[0]=p->wcs->cd[0]; w[1]=p->wcs->cd[1]; w[2]=p->wcs->cd[2]; w[3]=p->wcs->cd[3]; } else error(EXIT_FAILURE, 0, "currently the `--align' option only recognizes " "PCi_ja and CDi_ja keywords, not any others"); /* Find the pixel scale along the two dimensions. Note that we will be using the scale along the image X axis for both values. */ gal_wcs_pixel_scale_deg(p->wcs, &dx, &dy); /* Lets call the given WCS orientation `W', the rotation matrix we want to find as `X' and the final (aligned matrix) to have just one useful value: `a' (which is the pixel scale): x0 x1 w0 w1 -a 0 x2 x3 * w2 w3 = 0 a Let's open up the matrix multiplication, so we can find the `X' elements as function of the `W' elements and `a'. x0*w0 + x1*w2 = -a (1) x0*w1 + x1*w3 = 0 (2) x2*w0 + x3*w2 = 0 (3) x2*w1 + x3*w3 = a (4) Let's bring the X with the smaller index in each equation to the left side: x0 = (-w2/w0)*x1 - a/w0 (5) x0 = (-w3/w1)*x1 (6) x2 = (-w2/w0)*x3 (7) x2 = (-w3/w1)*x3 + a/w1 (8) Using (5) and (6) we can find x0 and x1, by first eliminating x0: (-w2/w0)*x1 - a/w0 = (-w3/w1)*x1 -> (w3/w1 - w2/w0) * x1 = a/w0 For easy reading/writing, let's define: A = (w3/w1 - w2/w0) --> x1 = a / w0 / A --> x0 = -1 * x1 * w3 / w1 Similar to the above, we can find x2 and x3 from (7) and (8): (-w2/w0)*x3 = (-w3/w1)*x3 + a/w1 -> (w3/w1 - w2/w0) * x3 = a/w1 --> x3 = a / w1 / A --> x2 = -1 * x3 * w2 / w0 Note that when the image is already aligned, a unity matrix should be output. */ if( w[1]==0.0f && w[2]==0.0f ) { amatrix[0]=1.0f; amatrix[1]=0.0f; amatrix[2]=0.0f; amatrix[3]=1.0f; } else { A = (w[3]/w[1]) - (w[2]/w[0]); amatrix[1] = dx / w[0] / A; amatrix[3] = dx / w[1] / A; amatrix[0] = -1 * amatrix[1] * w[3] / w[1]; amatrix[2] = -1 * amatrix[3] * w[2] / w[0]; } /* For a check: printf("dx: %e\n", dx); printf("w:\n"); printf(" %.8e %.8e\n", w[0], w[1]); printf(" %.8e %.8e\n", w[2], w[3]); printf("x:\n"); printf(" %.8e %.8e\n", amatrix[0], amatrix[1]); printf(" %.8e %.8e\n", amatrix[2], amatrix[3]); */ /* Put the matrix elements into the output array: */ tmatrix[0]=amatrix[0]; tmatrix[1]=amatrix[1]; tmatrix[2]=0.0f; tmatrix[3]=amatrix[2]; tmatrix[4]=amatrix[3]; tmatrix[5]=0.0f; tmatrix[6]=0.0f; tmatrix[7]=0.0f; tmatrix[8]=1.0f; } /**************************************************************/ /*************** Prepare Matrix *******************/ /**************************************************************/ /* This function is mainly for easy checking/debugging. */ void printmatrix(double *matrix) { printf("%-10.3f%-10.3f%-10.3f\n", matrix[0], matrix[1], matrix[2]); printf("%-10.3f%-10.3f%-10.3f\n", matrix[3], matrix[4], matrix[5]); printf("%-10.3f%-10.3f%-10.3f\n", matrix[6], matrix[7], matrix[8]); } void inplace_matrix_multiply(double *in, double *with) { /* `tin' will keep the values of the input array because we want to write the multiplication result in the input array. */ double tin[9]={in[0],in[1],in[2],in[3],in[4],in[5],in[6],in[7],in[8]}; /* For easy checking, here are the matrix/memory layouts: tin[0] tin[1] tin[2] with[0] with[1] with[2] tin[3] tin[4] tin[5] * with[3] with[4] with[5] tin[6] tin[7] tin[8] with[6] with[7] with[8] */ in[0] = tin[0]*with[0] + tin[1]*with[3] + tin[2]*with[6]; in[1] = tin[0]*with[1] + tin[1]*with[4] + tin[2]*with[7]; in[2] = tin[0]*with[2] + tin[1]*with[5] + tin[2]*with[8]; in[3] = tin[3]*with[0] + tin[4]*with[3] + tin[5]*with[6]; in[4] = tin[3]*with[1] + tin[4]*with[4] + tin[5]*with[7]; in[5] = tin[3]*with[2] + tin[4]*with[5] + tin[5]*with[8]; in[6] = tin[6]*with[0] + tin[7]*with[3] + tin[8]*with[6]; in[7] = tin[6]*with[1] + tin[7]*with[4] + tin[8]*with[7]; in[8] = tin[6]*with[2] + tin[7]*with[5] + tin[8]*with[8]; } /* Fill in the warping matrix elements based on the options/arguments */ void prepare_modular_matrix(struct imgwarpparams *p) { int f1, f2; /* For flipping. */ double s, c, tmatrix[9]; struct uiparams *up=&p->up; struct optionwarpsll *tmp, *next; /* Allocate space for the matrix, then initialize it. */ p->matrix[0]=1.0f; p->matrix[1]=0.0f; p->matrix[2]=0.0f; p->matrix[3]=0.0f; p->matrix[4]=1.0f; p->matrix[5]=0.0f; p->matrix[6]=0.0f; p->matrix[7]=0.0f; p->matrix[8]=1.0f; /* The linked list is last-in-first-out, so we need to reverse it to easily apply the changes in the same order that was read in. */ prepare_optionwapsll(p); /* Do all the operations */ tmp=up->owll; while(tmp!=NULL) { /* Fill `tmatrix' depending on the type of the warp. */ switch(tmp->type) { case ALIGN_WARP: makealignmatrix(p, tmatrix); break; case ROTATE_WARP: s = sin( tmp->v1*M_PI/180 ); c = cos( tmp->v1*M_PI/180 ); tmatrix[0]=c; tmatrix[1]=s; tmatrix[2]=0.0f; tmatrix[3]=-1.0f*s; tmatrix[4]=c; tmatrix[5]=0.0f; tmatrix[6]=0.0f; tmatrix[7]=0.0f; tmatrix[8]=1.0f; break; case SCALE_WARP: if( isnan(tmp->v2) ) tmp->v2=tmp->v1; tmatrix[0]=tmp->v1; tmatrix[1]=0.0f; tmatrix[2]=0.0f; tmatrix[3]=0.0f; tmatrix[4]=tmp->v2; tmatrix[5]=0.0f; tmatrix[6]=0.0f; tmatrix[7]=0.0f; tmatrix[8]=1.0f; break; case FLIP_WARP: /* For the flip, the values dont really matter! As long as the value is non-zero, the flip in the respective axis will be made. Note that the second axis is optional (can be NaN), but the first axis is required.*/ f1 = tmp->v1==0.0f ? 0 : 1; f2 = isnan(tmp->v2) ? 0 : ( tmp->v2==0.0f ? 0 : 1); if( f1 && !f2 ) { tmatrix[0]=1.0f; tmatrix[1]=0.0f; tmatrix[3]=0.0f; tmatrix[4]=-1.0f; } else if ( !f1 && f2 ) { tmatrix[0]=-1.0f; tmatrix[1]=0.0f; tmatrix[3]=0.0f; tmatrix[4]=1.0f; } else { tmatrix[0]=-1.0f; tmatrix[1]=0.0f; tmatrix[3]=0.0f; tmatrix[4]=-1.0f; } tmatrix[2]=0.0f; tmatrix[5]=0.0f; tmatrix[6]=0.0f; tmatrix[7]=0.0f; tmatrix[8]=1.0f; break; case SHEAR_WARP: if( isnan(tmp->v2) ) tmp->v2=tmp->v1; tmatrix[0]=1.0f; tmatrix[1]=tmp->v1; tmatrix[2]=0.0f; tmatrix[3]=tmp->v2; tmatrix[4]=1.0f; tmatrix[5]=0.0f; tmatrix[6]=0.0f; tmatrix[7]=0.0f; tmatrix[8]=1.0f; break; case TRANSLATE_WARP: if( isnan(tmp->v2) ) tmp->v2=tmp->v1; tmatrix[0]=1.0f; tmatrix[1]=0.0f; tmatrix[2]=tmp->v1; tmatrix[3]=0.0f; tmatrix[4]=1.0f; tmatrix[5]=tmp->v2; tmatrix[6]=0.0f; tmatrix[7]=0.0f; tmatrix[8]=1.0f; break; case PROJECT_WARP: if( isnan(tmp->v2) ) tmp->v2=tmp->v1; tmatrix[0]=1.0f; tmatrix[1]=0.0f; tmatrix[2]=0.0f; tmatrix[3]=0.0f; tmatrix[4]=1.0f; tmatrix[5]=0.0f; tmatrix[6]=tmp->v1; tmatrix[7]=tmp->v2; tmatrix[8]=1.0f; break; default: error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we can " "address the problem. For some reason the value of tmp->type " "in `prepare_modular_matrix' of ui.c is not recognized. " "This is an internal, not a user issue. So please let us " "know.", PACKAGE_BUGREPORT); } /* Multiply this matrix with the main matrix in-place. */ inplace_matrix_multiply(p->matrix, tmatrix); /* Keep the next element and free the node's allocated space. */ next = tmp->next; free(tmp); tmp = next; /* For a check: printf("tmatrix:\n"); printmatrix(tmatrix); printf("out:\n"); printmatrix(p->matrix); */ } } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ void sanitycheck(struct imgwarpparams *p) { double *d, *df, *m=p->matrix; /* Make sure the input file exists. */ gal_checkset_check_file(p->up.inputname); /* Set the output name: */ if(p->cp.output) gal_checkset_check_remove_file(p->cp.output, p->cp.dontdelete); else gal_checkset_automatic_output(p->up.inputname, "_warped.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->cp.output); /* If an actual matrix is given, then it will be used and all modular warpings will be ignored. */ if(p->up.matrixstring || p->up.matrixname) read_matrix(p); else if (p->up.owll) prepare_modular_matrix(p); else error(EXIT_FAILURE, 0, "No input matrix specified.\n\nPlease either " "use the modular warp options like `--rotate' or `--scale', " "or directly specify the matrix on the command-line, or in the " "configuration files.\n\nRun with `--help' for the full list of " "modular warpings (among other options), or see the manual's " "`Warping basics' section for more on the matrix."); /* Check if there are any non-normal numbers in the matrix: */ df=(d=p->matrix)+9; do if(!isfinite(*d++)) { printmatrix(p->matrix); error(EXIT_FAILURE, 0, "%f is not a `normal' number in the " "input matrix shown above", *(d-1)); } while(dmatrix; /* Read in the input image: */ numnul=gal_fits_hdu_to_array(p->up.inputname, p->cp.hdu, &p->inputbitpix, &array, &p->is0, &p->is1); if(p->inputbitpix==DOUBLE_IMG) p->input=array; else { gal_fits_change_type(array, p->inputbitpix, p->is0*p->is1, numnul, (void **)&p->input, DOUBLE_IMG); free(array); } /* Make the inverse matrix: */ errno=0; p->inverse=inv=malloc(9*sizeof *inv); if(inv==NULL) error(EXIT_FAILURE, errno, "%zu bytes for the inverse array", 9*sizeof *inv); inv[0]=m[4]*m[8]-m[5]*m[7]; inv[1]=m[2]*m[7]-m[1]*m[8]; inv[2]=m[1]*m[5]-m[2]*m[4]; inv[3]=m[5]*m[6]-m[3]*m[8]; inv[4]=m[0]*m[8]-m[2]*m[6]; inv[5]=m[2]*m[3]-m[0]*m[5]; inv[6]=m[3]*m[7]-m[4]*m[6]; inv[7]=m[1]*m[6]-m[0]*m[7]; inv[8]=m[0]*m[4]-m[1]*m[3]; /* Just for a test: { size_t i; printf("\nInput matrix:"); for(i=0;i<9;++i) { if(i%3==0) printf("\n"); printf("%-10.5f", m[i]); } printf("\n-----------\n"); printf("Inverse matrix:"); for(i=0;i<9;++i) { if(i%3==0) printf("\n"); printf("%-10.5f", inv[i]); } printf("\n\n"); } */ } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void setparams(int argc, char *argv[], struct imgwarpparams *p) { struct gal_commonparams *cp=&p->cp; /* Set the non-zero initial values, the structure was initialized to have a zero value for all elements. */ cp->spack = SPACK; cp->verb = 1; cp->numthreads = num_processors(NPROC_CURRENT); cp->removedirinfo = 1; p->correctwcs = 1; p->up.owll = NULL; /* Read the arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Add the user default values and save them if asked. */ GAL_CONFIGFILES_CHECK_SET_CONFIG; /* Check if all the required parameters are set. */ checkifset(p); /* Print the values for each parameter. */ if(cp->printparams) GAL_CONFIGFILES_REPORT_PARAMETERS_SET; /* Read the input image WCS structure. We are doing this here because some of the matrix operations might need it. */ gal_fits_read_wcs(p->up.inputname, p->cp.hdu, p->hstartwcs, p->hendwcs, &p->nwcs, &p->wcs); /* Do a sanity check. */ sanitycheck(p); gal_checkset_check_remove_file(GAL_TXTARRAY_LOG, 0); /* Everything is ready, notify the user of the program starting. */ if(cp->verb) { printf(SPACK_NAME" started on %s", ctime(&p->rawtime)); printf(" Using %zu CPU thread%s\n", p->cp.numthreads, p->cp.numthreads==1 ? "." : "s."); printf(" Input image: %s\n", p->up.inputname); printf(" matrix:" "\n\t%.4f %.4f %.4f" "\n\t%.4f %.4f %.4f" "\n\t%.4f %.4f %.4f\n", p->matrix[0], p->matrix[1], p->matrix[2], p->matrix[3], p->matrix[4], p->matrix[5], p->matrix[6], p->matrix[7], p->matrix[8]); } /* Make the array of input images. */ preparearrays(p); } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void freeandreport(struct imgwarpparams *p, struct timeval *t1) { /* Free the allocated arrays: */ free(p->input); free(p->cp.hdu); free(p->inverse); free(p->cp.output); if(p->wcs) wcsvfree(&p->nwcs, &p->wcs); /* Print the final message. */ if(p->cp.verb) gal_timing_report(t1, SPACK_NAME" finished in: ", 0); } gnuastro-0.2.33-8a3b/bin/imgwarp/cite.h0000644000175000017500000000316412750745735014453 00000000000000/********************************************************************* ImageWarp - Warp images using projective mapping. ImageWarp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CITE_H #define CITE_H #define IMGWARPBIBTEX "" #define PRINTCITEABORT { \ printf("\nWe hope %s has been useful for your research.\n" \ "Citations are vital for the continued work on %s.\n" \ "Thank you for citing it in your research paper.\n" \ "\nPlease cite as \"%s\":\n\n%s\n\n%s", \ SPACK_NAME, SPACK_NAME, SPACK_STRING, \ GAL_STRINGS_MAIN_BIBTEX, IMGWARPBIBTEX); \ exit(EXIT_SUCCESS); \ } #endif gnuastro-0.2.33-8a3b/bin/imgwarp/main.h0000644000175000017500000000773313002470065014437 00000000000000/********************************************************************* ImageWarp - Warp images using projective mapping. ImageWarp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include #include /* Progarm name macros: */ #define SPACK "astimgwarp" /* Subpackage executable name. */ #define SPACK_NAME "ImageWarp" /* Subpackage full name. */ #define SPACK_STRING SPACK_NAME" ("PACKAGE_NAME") "PACKAGE_VERSION #define LOGFILENAME SPACK".log" struct optionwarpsll { int type; double v1; double v2; struct optionwarpsll *next; }; struct uiparams { char *inputname; /* Name of input file. */ char *matrixname; /* Name of transform file. */ char *matrixstring; /* String containing transform elements. */ struct optionwarpsll *owll; /* List of 2D rotations. */ int nofitscorrect; /* No corr the 0.5 pixel necessary in FITS. */ int nofitscorrectset; int matrixstringset; int maxblankfracset; int hstartwcsset; int hendwcsset; }; struct imgwarpparams { /* Other structures: */ struct uiparams up; /* User interface parameters. */ struct gal_commonparams cp; /* Common parameters. */ /* Input: */ double *input; /* Name of input FITS file. */ double matrix[9]; /* Warp/Transformation matrix. */ size_t is0; /* Number of rows in input image. */ size_t is1; /* Number of columns in input image. */ int inputbitpix; /* The type of the input array. */ int nwcs; /* Number of WCS structures. */ struct wcsprm *wcs; /* Pointer to WCS structures. */ size_t hstartwcs; /* Header keyword No. to start reading WCS. */ size_t hendwcs; /* Header keyword No. to end reading WCS. */ /* Output: */ size_t numnul; /* Number of blank pixels in output. */ int correctwcs; /* Wrap the warped/transfomed pixels. */ int doubletype; /* Save output in double not in input type. */ int zerofornoinput; /* Set the pixels with no input to zero. */ float maxblankfrac; /* Maximum fraction of blank pixel in out. */ /* Internal parameters: */ double *output; /* Warped image array. */ size_t onaxes[2]; /* Output image size */ size_t knaxes[2]; /* Output image size */ double *inverse; /* Inverse of the input matrix. */ time_t rawtime; /* Starting time of the program. */ size_t extinds[4]; /* Indexs of the minimum and maximum values. */ size_t ordinds[4]; /* Indexs of anticlockwise vertices. */ double outfpixval[2]; /* Pixel value of first output pixel. */ double opixarea; /* Area of output pix in units of input pix. */ }; #endif gnuastro-0.2.33-8a3b/bin/imgwarp/main.c0000644000175000017500000000322012774157256014440 00000000000000/********************************************************************* ImageWarp - Warp images using projective mapping. ImageWarp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include /* Includes time.h and sys/time.h */ #include "main.h" #include "ui.h" /* Needs main.h. */ #include "imgwarp.h" /* Needs main.h. */ int main (int argc, char *argv[]) { struct timeval t1; struct imgwarpparams p={{0}, {0}, 0}; /* Set the starting time.*/ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ setparams(argc, argv, &p); /* Run ImageWarp */ imgwarp(&p); /* Free all non-freed allocations. */ freeandreport(&p, &t1); /* Return successfully.*/ return EXIT_SUCCESS; } gnuastro-0.2.33-8a3b/bin/imgwarp/Makefile.in0000644000175000017500000017251713004464626015422 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or 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GNULIB_BTOWC = @GNULIB_BTOWC@ GNULIB_CALLOC_POSIX = @GNULIB_CALLOC_POSIX@ GNULIB_CANONICALIZE_FILE_NAME = @GNULIB_CANONICALIZE_FILE_NAME@ GNULIB_CBRT = @GNULIB_CBRT@ GNULIB_CBRTF = @GNULIB_CBRTF@ GNULIB_CBRTL = @GNULIB_CBRTL@ GNULIB_CEIL = @GNULIB_CEIL@ GNULIB_CEILF = @GNULIB_CEILF@ GNULIB_CEILL = @GNULIB_CEILL@ GNULIB_CHDIR = @GNULIB_CHDIR@ GNULIB_CHOWN = @GNULIB_CHOWN@ GNULIB_CLOSE = @GNULIB_CLOSE@ GNULIB_COPYSIGN = @GNULIB_COPYSIGN@ GNULIB_COPYSIGNF = @GNULIB_COPYSIGNF@ GNULIB_COPYSIGNL = @GNULIB_COPYSIGNL@ GNULIB_COSF = @GNULIB_COSF@ GNULIB_COSHF = @GNULIB_COSHF@ GNULIB_COSL = @GNULIB_COSL@ GNULIB_DPRINTF = @GNULIB_DPRINTF@ GNULIB_DUP = @GNULIB_DUP@ GNULIB_DUP2 = @GNULIB_DUP2@ GNULIB_DUP3 = @GNULIB_DUP3@ GNULIB_DUPLOCALE = @GNULIB_DUPLOCALE@ GNULIB_ENVIRON = @GNULIB_ENVIRON@ GNULIB_EUIDACCESS = @GNULIB_EUIDACCESS@ GNULIB_EXP2 = @GNULIB_EXP2@ GNULIB_EXP2F = @GNULIB_EXP2F@ GNULIB_EXP2L = @GNULIB_EXP2L@ GNULIB_EXPF = @GNULIB_EXPF@ GNULIB_EXPL = @GNULIB_EXPL@ GNULIB_EXPM1 = @GNULIB_EXPM1@ GNULIB_EXPM1F = @GNULIB_EXPM1F@ GNULIB_EXPM1L = @GNULIB_EXPM1L@ GNULIB_FABSF = @GNULIB_FABSF@ GNULIB_FABSL = @GNULIB_FABSL@ GNULIB_FACCESSAT = @GNULIB_FACCESSAT@ GNULIB_FCHDIR = @GNULIB_FCHDIR@ GNULIB_FCHMODAT = @GNULIB_FCHMODAT@ GNULIB_FCHOWNAT = @GNULIB_FCHOWNAT@ GNULIB_FCLOSE = @GNULIB_FCLOSE@ GNULIB_FCNTL = @GNULIB_FCNTL@ GNULIB_FDATASYNC = @GNULIB_FDATASYNC@ GNULIB_FDOPEN = @GNULIB_FDOPEN@ GNULIB_FFLUSH = @GNULIB_FFLUSH@ GNULIB_FFS = @GNULIB_FFS@ GNULIB_FFSL = @GNULIB_FFSL@ GNULIB_FFSLL = @GNULIB_FFSLL@ GNULIB_FGETC = @GNULIB_FGETC@ GNULIB_FGETS = @GNULIB_FGETS@ GNULIB_FLOOR = @GNULIB_FLOOR@ GNULIB_FLOORF = @GNULIB_FLOORF@ GNULIB_FLOORL = @GNULIB_FLOORL@ GNULIB_FMA = @GNULIB_FMA@ GNULIB_FMAF = @GNULIB_FMAF@ GNULIB_FMAL = @GNULIB_FMAL@ GNULIB_FMOD = @GNULIB_FMOD@ GNULIB_FMODF = @GNULIB_FMODF@ GNULIB_FMODL = @GNULIB_FMODL@ GNULIB_FOPEN = @GNULIB_FOPEN@ GNULIB_FPRINTF = @GNULIB_FPRINTF@ GNULIB_FPRINTF_POSIX = @GNULIB_FPRINTF_POSIX@ GNULIB_FPURGE = @GNULIB_FPURGE@ GNULIB_FPUTC = @GNULIB_FPUTC@ GNULIB_FPUTS = @GNULIB_FPUTS@ GNULIB_FREAD = @GNULIB_FREAD@ GNULIB_FREOPEN = @GNULIB_FREOPEN@ GNULIB_FREXP = @GNULIB_FREXP@ GNULIB_FREXPF = @GNULIB_FREXPF@ GNULIB_FREXPL = @GNULIB_FREXPL@ GNULIB_FSCANF = @GNULIB_FSCANF@ GNULIB_FSEEK = @GNULIB_FSEEK@ GNULIB_FSEEKO = @GNULIB_FSEEKO@ GNULIB_FSTAT = @GNULIB_FSTAT@ GNULIB_FSTATAT = @GNULIB_FSTATAT@ GNULIB_FSYNC = @GNULIB_FSYNC@ GNULIB_FTELL = @GNULIB_FTELL@ GNULIB_FTELLO = @GNULIB_FTELLO@ GNULIB_FTRUNCATE = @GNULIB_FTRUNCATE@ GNULIB_FUTIMENS = @GNULIB_FUTIMENS@ GNULIB_FWRITE = @GNULIB_FWRITE@ GNULIB_GETC = @GNULIB_GETC@ GNULIB_GETCHAR = @GNULIB_GETCHAR@ GNULIB_GETCWD = @GNULIB_GETCWD@ GNULIB_GETDELIM = @GNULIB_GETDELIM@ GNULIB_GETDOMAINNAME = @GNULIB_GETDOMAINNAME@ GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = 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.NOEXPORT: gnuastro-0.2.33-8a3b/bin/imgwarp/astimgwarp.conf0000644000175000017500000000141313002470065016354 00000000000000# Default parameters (System) for ImageWarp. # ImageWarp is part of GNU Astronomy Utitlies. # # Use the long option name of each paramter followed by # a value. The name and value should be separated by # atleast one of the following charaacters: # space, `,`, `=` or `:` # # Run with `--help` option or read the manual for a full # explanation of what each option means. # # NOTE I: All counting is from zero, not one. # NOTE II: Lines starting with `#` are ignored. # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Input: hdu 0 # Output: scale 1.0 maxblankfrac 0.8gnuastro-0.2.33-8a3b/bin/imgwarp/Makefile.am0000644000175000017500000000270012765246727015410 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. NOTE: $(top_srcdir)/bootstrapped/lib is only necessary ## for internally compiled utilities and libraries. It must not be included ## during the tests since the bootstrapped libraries are not installed. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Utility and its sources bin_PROGRAMS = astimgwarp astimgwarp_SOURCES = main.c main.h cite.h ui.c ui.h args.h \ imgwarp.c imgwarp.h astimgwarp_LDADD = $(top_builddir)/bootstrapped/lib/libgnu.la \ -lgnuastro ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astimgwarp.conf gnuastro-0.2.33-8a3b/bin/imgstat/0000755000175000017500000000000013004464724013421 500000000000000gnuastro-0.2.33-8a3b/bin/imgstat/imgstat.h0000644000175000017500000000210212616616510015155 00000000000000/********************************************************************* ImageStatistics - Get general statistics about the image. ImgeStatistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef IMGSTAT_H #define IMGSTAT_H void imgstat(struct imgstatparams *p); #endif gnuastro-0.2.33-8a3b/bin/imgstat/imgstat.c0000644000175000017500000002317513001632537015161 00000000000000/********************************************************************* ImageStatistics - Get general statistics about the image. ImgeStatistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include "main.h" #include "imgstat.h" /* This function will report the simple immediate statistics of the data. For the average and standard deviation, the unsorted data is used so we don't suddenly encounter rounding errors. */ void reportsimplestats(struct imgstatparams *p) { double sum; size_t modeindex; float modequant, symvalue; float ave, std, med, modesym; sum=gal_statistics_float_sum(p->img, p->size); gal_statistics_f_ave_std(p->img, p->size, &ave, &std, NULL); med=p->sorted[gal_statistics_index_from_quantile(p->size, 0.5f)]; /* Very simple and basic: */ printf(SNAMEVAL FNAMEVAL FNAMEVAL, "Number of points", p->size, "Minimum", p->sorted[0], "Maximum", p->sorted[p->size-1]); printf(FNAMEVAL FNAMEVAL FNAMEVAL FNAMEVAL, "Sum", sum, "Mean", ave, "Standard deviation", std, "Median", med); /* The mode: */ gal_statistics_mode_index_in_sorted(p->sorted, p->size, p->mirrordist, &modeindex, &modesym); modequant=(float)(modeindex)/(float)(p->size); /* Report the values: */ printf(" -- %-45s%.4f %g\n", "Mode (quantile, value)", modequant, p->sorted[modeindex]); symvalue=gal_statistics_mode_value_from_sym(p->sorted, p->size, modeindex, modesym); printf(" -- %-45s%.4f %g\n", "Mode symmetricity and its cutoff" " value", modesym, symvalue); if(modesymmhistname) gal_statistics_mode_mirror_plots(p->sorted, p->size, modeindex, p->histmin, p->histmax, p->histnumbins, p->mhistname, p->mcfpname, (p->histrangeformirror ? 0.0f : p->mirrorplotdist) ); } void printasciihist(struct imgstatparams *p) { size_t j; float *bins; float quant=-1.0f; /* histmin and histmax were already set before. */ int i, binonzero=0, normhist=0, maxhistone=1; /* Find the histogram for the ASCII plot: */ gal_statistics_set_bins(p->sorted, p->size, ASCIIHISTNUMBINS, p->histmin, p->histmax, binonzero, quant, &bins); gal_statistics_histogram(p->sorted, p->size, bins, ASCIIHISTNUMBINS, normhist, maxhistone); /* It's maximum value is set to one. Multiply that by the desired height in pixels. */ for(j=0;jhistmin, p->histmax); for(i=ASCIIHISTHEIGHT;i>=0;--i) { printf(" |"); for(j=0;j=((float)i-0.5f) && bins[j*2+1]>0.0f) printf("*"); else printf(" "); } printf("\n"); } printf(" |"); for(j=0;jup.inputname, p->cp.hdu); if(p->up.masknameset) fprintf(out, "# Mask (hdu): %s (%s)\n", p->up.maskname, p->up.mhdu); if(p->lowerbin) fprintf(out, "# Column 1: Flux of lower value of each bin\n"); else fprintf(out, "# Column 1: Flux in the middle of each bin\n"); if(strcmp(outputtype, CFPSTRING)==0) { fprintf(out, "# Column 2: Average of the sorted index of all points " "in this bin"); if(p->normcfp) fprintf(out, " (normalized).\n"); else if (p->maxcfpeqmaxhist) fprintf(out, " (Scaled to the histogram).\n"); else { fprintf(out, ".\n"); int0float1=0; } } else if (strcmp(outputtype, HISTSTRING)==0) { if(p->normhist) fprintf(out, "# Column 2: Fraction of points in this bin. \n"); else if(p->maxhistone) fprintf(out, "# Column 2: Histogram if the maximum bin is " "set to 1.\n"); else { fprintf(out, "# Column 2: Number of points in this bin. \n"); int0float1=0; } } /* Put the data in the file: */ if(p->lowerbin==0) d=(bins[2]-bins[0])/2; else d=0.0f; if(int0float1) for(i=0;icp.verb) { reportsimplestats(p); if(p->asciihist) printasciihist(p); } /* Make the histogram: */ if(p->histname) { /* Make the actual data histogram and save it. */ gal_statistics_set_bins(p->sorted, p->size, p->histnumbins, p->histmin, p->histmax, p->onebinvalue, quant, &bins); gal_statistics_histogram(p->sorted, p->size, bins, p->histnumbins, p->normhist, p->maxhistone); printhistcfp(p, bins, p->histnumbins, p->histname, HISTSTRING); /* Get the hisogram maximum value if it is needed for the cumulative frequency plot. */ if(p->maxcfpeqmaxhist) for(i=0;ihistnumbins;++i) if(bins[i*2+1]>maxhist) maxhist=bins[i*2+1]; } /* Make the cumulative distribution function: */ if(p->cfpname) { if(p->cfpsimhist) { p->cfpnum=p->histnumbins; for(i=0;icfpnum;++i) bins[i*2+1]=0.0f; } else { if(p->histname) free(bins); gal_statistics_set_bins(p->sorted, p->size, p->cfpnum, p->cfpmin, p->cfpmax, p->onebinvalue, quant, &bins); } gal_statistics_cumulative_fp(p->sorted, p->size, bins, p->cfpnum, p->normcfp); if(p->maxcfpeqmaxhist) for(i=0;icfpnum;++i) bins[i*2+1]*=(maxhist/p->size); printhistcfp(p, bins, p->cfpnum, p->cfpname, CFPSTRING); } /* Make the mirror distribution if asked for: */ if(isnan(p->mirror)==0) gal_statistics_mode_mirror_plots(p->sorted, p->size, gal_statistics_index_from_quantile(p->size, p->mirror), p->histmin, p->histmax, p->histnumbins, p->mirrorhist, p->mirrorcfp, (p->histrangeformirror ? 0.0f : p->mirrorplotdist)); /* Print out the Sigma clippings: */ if(p->sigclip && p->cp.verb) { printf(" - Sigma clipping results (Median, Mean, STD, Number):\n"); printf(" - %.2f times sigma by convergence (tolerance: %.4f):\n", p->sigclipmultip, p->sigcliptolerance); r=gal_statistics_sigma_clip_converge(p->sorted, 1, p->size, p->sigclipmultip, p->sigcliptolerance, &ave, &med, &std, 1); if(r==0) printf(" #### Could not converge\n"); printf(" - %.2f sigma-clipping %zu times:\n", p->sigclipmultip, p->sigclipnum); gal_statistics_sigma_clip_certain_num(p->sorted, 1, p->size, p->sigclipmultip, p->sigclipnum, &ave, &med, &std, 1); } /* Free the allocated arrays: */ if(p->histname || p->cfpname) free(bins); } gnuastro-0.2.33-8a3b/bin/imgstat/args.h0000644000175000017500000002720012774160533014453 00000000000000/********************************************************************* ImageStatistics - Get general statistics about the image. ImgeStatistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef ARGS_H #define ARGS_H #include #include #include #include /**************************************************************/ /************** argp.h definitions ***************/ /**************************************************************/ /* Definition parameters for the argp: */ const char *argp_program_version=SPACK_STRING"\n"GAL_STRINGS_COPYRIGHT "\n\nWritten by Mohammad Akhlaghi"; const char *argp_program_bug_address=PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata"; const char doc[] = /* Before the list of options: */ GAL_STRINGS_TOP_HELP_INFO SPACK_NAME" will print the basic statistics of the input image pixel " "flux distribution. All blank pixels or pixels specified by a mask " "image will be ignored.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /* Available letters for short options: c e f j k m s t v w y z C E F G I J L O R T W X Y Z Number keys used: <=511 Options with keys (second structure element) larger than 500 do not have a short version. */ static struct argp_option options[] = { { 0, 0, 0, 0, "Input:", 1 }, { "mask", 'M', "STR", 0, "Mask image file name.", 1 }, { "mhdu", 'H', "STR", 0, "Mask image header name.", 1 }, { "ignoremin", 'r', 0, 0, "Ignore data with values equal to minimum.", 1 }, { "mirrordist", 'd', "FLT", 0, "Distance beyond mirror point. Multiple of std.", 1 }, { 0, 0, 0, 0, "Output:", 2 }, { "lowerbin", 'l', 0, 0, "Interval lower limit for column 1.", 2 }, { "onebinvalue", 'B', "FLT", 0, "Shift bins so one bin starts on this value.", 2 }, { "noasciihist", 'A', 0, 0, "Do not show an ASCII histogram of the data.", 2 }, { "checkmode", 509, 0, 0, "Mode mirror plot. `_modehist.txt', `_modecfp.txt'", 2 }, { "mirrorquant", 510, "FLT", 0, "Mirror quantile. `_mirhist.txt', `_mircfp.txt'.", 2 }, { "histrangeformirror", 511, 0, 0, "Use input histogram range for mirror plots.", 2 }, { "mirrorplotdist", 503, "FLT", 0, "Distance beyond mode to display.", 2 }, { 0, 0, 0, 0, "Histogram (suffix: `_hist.txt'):", 3 }, { "nohist", 500, 0, 0, "Do not calculate histogram.", 3 }, { "normhist", 501, 0, 0, "Normalize the histogram (sum of all bins 1).", 3 }, { "maxhistone", 502, 0, 0, "Scale such that the maximum bin has value of one.", 3 }, { "histnumbins", 'n', "INT", 0, "Number of bins in the histogram.", 3 }, { "histmin", 'i', "FLT", 0, "The minimum value for the histogram.", 3 }, { "histmax", 'x', "FLT", 0, "The maximum value for the histogram.", 3 }, { "histquant", 'Q', "FLT", 0, "Quantile (Q) range. Histogram from Q to 1-Q.", 3 }, { 0, 0, 0, 0, "Cumulative Frequency Plot (suffix: `_cfp.txt'):", 4 }, { "nocfp", 504, 0, 0, "No Cumulative Frequency Plot.", 4 }, { "normcfp", 505, 0, 0, "Normalize the CFP (sum of all bins 1).", 4 }, { "maxcfpeqmaxhist", 506, 0, 0, "Set maximum of CFP to maximum of histogram.", 4 }, { "cfpsimhist", 507, 0, 0, "Set CFP range and bins similar to histogram.", 4 }, { "cfpnum", 'p', "INT", 0, "Number of data points to find CFP.", 4 }, { "cfpmin", 'a', "FLT", 0, "Minimum value to use in the CFP.", 4 }, { "cfpmax", 'b', "FLT", 0, "Maximum value to use in the CFP.", 4 }, { "cfpquant", 'U', "FLT", 0, "Quantile of range: from U to 1-U.", 4 }, { 0, 0, 0, 0, "Sigma clipping:", 5 }, { "nosigclip", 508, 0, 0, "Do not preform sigma clipping.", 5 }, { "sigclipmultip", 'u', "FLT", 0, "Multiple of standard deviation in sigma-clipping.", 5 }, { "sigcliptolerance", 't', "FLT", 0, "Difference in STD tolerance to halt iteration.", 5 }, { "sigclipnum", 'g', "INT", 0, "Number of times to do sigma clipping.", 5 }, { 0, 0, 0, 0, "Operating modes:", -1 }, {0} }; /* Parse a single option: */ static error_t parse_opt(int key, char *arg, struct argp_state *state) { /* Save the arguments structure: */ struct imgstatparams *p = state->input; /* Set the pointer to the common parameters for all programs here: */ state->child_inputs[0]=&p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); switch(key) { /* Input: */ case 'M': gal_checkset_allocate_copy_set(arg, &p->up.maskname, &p->up.masknameset); break; case 'H': gal_checkset_allocate_copy_set(arg, &p->up.mhdu, &p->up.mhduset); break; case 'r': p->ignoremin=1; break; case 'd': gal_checkset_float_l_0(arg, &p->mirrordist, "mirrordist", key, SPACK, NULL, 0); p->up.mirrordistset=1; break; /* Output: */ case 'l': p->lowerbin=1; break; case 'B': gal_checkset_any_float(arg, &p->onebinvalue, "onebinvalue", key, SPACK, NULL, 0); p->up.onebinvalueset=1; break; case 'A': p->asciihist=0; break; case 509: p->mhistname="a"; break; case 510: gal_checkset_float_l_0_s_1(arg, &p->mirror, "mirrorquant", key, SPACK, NULL, 0); break; case 511: p->histrangeformirror=1; break; case 503: gal_checkset_float_l_0(arg, &p->mirrorplotdist, "mirrorplotdist", key, SPACK, NULL, 0); p->up.mirrorplotdistset=1; break; /* Histogram */ case 500: p->histname=NULL; break; case 501: p->normhist=1; break; case 502: p->maxhistone=1; break; case 'n': gal_checkset_sizet_l_zero(arg, &p->histnumbins, "histnumbins", key, SPACK, NULL, 0); p->up.histnumbinsset=1; break; case 'i': gal_checkset_any_float(arg, &p->histmin, "histmin", key, SPACK, NULL, 0); p->up.histminset=1; break; case 'x': gal_checkset_any_float(arg, &p->histmax, "histmax", key, SPACK, NULL, 0); p->up.histmaxset=1; break; case 'Q': gal_checkset_float_l_0_s_1(arg, &p->histquant, "histquant", key, SPACK, NULL, 0); p->up.histquantset=1; break; /* Cumulative frequency plot: */ case 504: p->cfpname=NULL; break; case 505: p->normcfp=1; break; case 506: p->maxcfpeqmaxhist=1; break; case 507: p->cfpsimhist=1; break; case 'p': gal_checkset_sizet_l_zero(arg, &p->cfpnum, "cfpnum", key, SPACK, NULL, 0); p->up.cfpnumset=1; break; case 'a': gal_checkset_any_float(arg, &p->cfpmin, "cfpmin", key, SPACK, NULL, 0); p->up.cfpminset=1; break; case 'b': gal_checkset_any_float(arg, &p->cfpmax, "cfpmax", key, SPACK, NULL, 0); p->up.cfpmaxset=1; break; case 'U': gal_checkset_float_l_0_s_1(arg, &p->cfpquant, "cfpquant", key, SPACK, NULL, 0); p->up.cfpquantset=1; break; /* Sigma clipping: */ case 508: p->sigclip=0; break; case 'u': gal_checkset_float_l_0(arg, &p->sigclipmultip, "sigclipmultip", key, SPACK, NULL, 0); p->up.sigclipmultipset=1; break; case 't': gal_checkset_float_l_0(arg, &p->sigcliptolerance, "sigcliptolerance", key, SPACK, NULL, 0); p->up.sigcliptoleranceset=1; break; case 'g': gal_checkset_sizet_l_zero(arg, &p->sigclipnum, "sigclipnum", key, SPACK, NULL, 0); p->up.sigclipnumset=1; break; /* Operating modes: */ /* Read the non-option arguments: */ case ARGP_KEY_ARG: /* See what type of input value it is and put it in. */ if( gal_fits_name_is_fits(arg) ) { if(p->up.inputname) argp_error(state, "only one input image should be given"); else p->up.inputname=arg; } else argp_error(state, "%s is not a valid file type", arg); break; /* The command line options and arguments are finished. */ case ARGP_KEY_END: if(p->cp.setdirconf==0 && p->cp.setusrconf==0 && p->cp.printparams==0) { if(state->arg_num==0) argp_error(state, "no argument given"); if(p->up.inputname==NULL) argp_error(state, "no input FITS image(s) provided"); } break; default: return ARGP_ERR_UNKNOWN; } return 0; } /* Specify the children parsers: */ struct argp_child children[]= { {&commonargp, 0, NULL, 0}, {0, 0, 0, 0} }; /* Basic structure defining the whole argument reading process. */ static struct argp thisargp = {options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif gnuastro-0.2.33-8a3b/bin/imgstat/ui.h0000644000175000017500000000224012616616510014125 00000000000000/********************************************************************* ImageStatistics - Get general statistics about the image. ImgeStatistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef IMCROPUI_H #define IMCROPUI_H void setparams(int argc, char *argv[], struct imgstatparams *p); void freeandreport(struct imgstatparams *p, struct timeval *t1); #endif gnuastro-0.2.33-8a3b/bin/imgstat/ui.c0000644000175000017500000005417313001632537014130 00000000000000/********************************************************************* ImageStatistics - Get general statistics about the image. ImgeStatistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include /* From Gnulib. */ #include /* Includes time.h and sys/time.h */ #include #include #include #include #include "main.h" #include "ui.h" /* Needs main.h */ #include "args.h" /* Needs main.h, includes argp.h. */ /* Set the file names of the places where the default parameters are put. */ #define CONFIG_FILE SPACK CONF_POSTFIX #define SYSCONFIG_FILE SYSCONFIG_DIR "/" CONFIG_FILE #define USERCONFIG_FILEEND USERCONFIG_DIR CONFIG_FILE #define CURDIRCONFIG_FILE CURDIRCONFIG_DIR CONFIG_FILE /**************************************************************/ /************** Options and parameters ***************/ /**************************************************************/ void readconfig(char *filename, struct imgstatparams *p) { FILE *fp; size_t lineno=0, len=200; char *line, *name, *value; struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; char key='a'; /* Not used, just a place holder. */ /* When the file doesn't exist or can't be opened, it is ignored. It might be intentional, so there is no error. If a parameter is missing, it will be reported after all defaults are read. */ fp=fopen(filename, "r"); if (fp==NULL) return; /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); /* Read the tokens in the file: */ while(getline(&line, &len, fp) != -1) { /* Prepare the "name" and "value" strings, also set lineno. */ GAL_CONFIGFILES_START_READING_LINE; /* Inputs: */ if(strcmp(name, "hdu")==0) gal_checkset_allocate_copy_set(value, &cp->hdu, &cp->hduset); else if (strcmp(name, "mask")==0) gal_checkset_allocate_copy_set(value, &up->maskname, &up->masknameset); else if (strcmp(name, "mhdu")==0) gal_checkset_allocate_copy_set(value, &up->mhdu, &up->mhduset); else if(strcmp(name, "mirrordist")==0) { if(up->mirrordistset) continue; gal_checkset_float_l_0(value, &p->mirrordist, name, key, SPACK, filename, lineno); up->mirrordistset=1; } /* Outputs */ else if(strcmp(name, "output")==0) gal_checkset_allocate_copy_set(value, &cp->output, &cp->outputset); else if(strcmp(name, "mirrorplotdist")==0) { if(up->mirrorplotdistset) continue; gal_checkset_float_l_0(value, &p->mirrorplotdist, name, key, SPACK, filename, lineno); up->mirrorplotdistset=1; } else if(strcmp(name, "onebinvalue")==0) { if(up->onebinvalueset) continue; gal_checkset_any_float(value, &p->onebinvalue, name, key, SPACK, filename, lineno); up->onebinvalueset=1; } /* Histogram: */ else if(strcmp(name, "histnumbins")==0) { if(up->histnumbinsset) continue; gal_checkset_sizet_l_zero(value, &p->histnumbins, name, key, SPACK, filename, lineno); up->histnumbinsset=1; } else if(strcmp(name, "histmin")==0) { if(up->histminset) continue; gal_checkset_any_float(value, &p->histmin, name, key, SPACK, filename, lineno); up->histminset=1; } else if(strcmp(name, "histmax")==0) { if(up->histmaxset) continue; gal_checkset_any_float(value, &p->histmax, name, key, SPACK, filename, lineno); up->histmaxset=1; } else if(strcmp(name, "histquant")==0) { if(up->histquantset) continue; gal_checkset_float_l_0_s_1(value, &p->histquant, name, key, SPACK, filename, lineno); up->histquantset=1; } /* Cumulative Frequency Plot: */ else if(strcmp(name, "cfpnum")==0) { if(up->cfpnumset) continue; gal_checkset_sizet_l_zero(value, &p->cfpnum, name, key, SPACK, filename, lineno); up->cfpnumset=1; } else if(strcmp(name, "cfpmin")==0) { if(up->cfpminset) continue; gal_checkset_any_float(value, &p->cfpmin, name, key, SPACK, filename, lineno); up->cfpminset=1; } else if(strcmp(name, "cfpmax")==0) { if(up->cfpmaxset) continue; gal_checkset_any_float(value, &p->cfpmax, name, key, SPACK, filename, lineno); up->cfpmaxset=1; } else if(strcmp(name, "cfpquant")==0) { if(up->cfpquantset) continue; gal_checkset_float_l_0_s_1(value, &p->cfpquant, name, key, SPACK, filename, lineno); up->cfpquantset=1; } /* Sigma clipping: */ else if(strcmp(name, "sigclipmultip")==0) { if(up->sigclipmultipset) continue; gal_checkset_float_l_0(value, &p->sigclipmultip, name, key, SPACK, filename, lineno); up->sigclipmultipset=1; } else if(strcmp(name, "sigcliptolerance")==0) { if(up->sigcliptoleranceset) continue; gal_checkset_float_l_0(value, &p->sigcliptolerance, name, key, SPACK, filename, lineno); up->sigcliptoleranceset=1; } else if(strcmp(name, "sigclipnum")==0) { if(up->sigclipnumset) continue; gal_checkset_sizet_l_zero(value, &p->sigclipnum, name, key, SPACK, filename, lineno); up->sigclipnumset=1; } /* Operating modes: */ /* Read options common to all programs */ GAL_CONFIGFILES_READ_COMMONOPTIONS_FROM_CONF else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s` not recognized.\n", name); } free(line); fclose(fp); } void printvalues(FILE *fp, struct imgstatparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; /* Print all the options that are set. Separate each group with a commented line explaining the options in that group. */ fprintf(fp, "\n# Input image:\n"); if(cp->hduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("hdu", cp->hdu); if(up->masknameset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("mask", up->maskname); if(up->mhdu) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("mhdu", up->mhdu); if(up->mirrordistset) fprintf(fp, CONF_SHOWFMT"%.2f\n", "mirrordist", p->mirrordist); /* Output: */ fprintf(fp, "\n# Output:\n"); if(cp->outputset) fprintf(fp, CONF_SHOWFMT"%s\n", "output", cp->output); if(up->mirrorplotdistset) fprintf(fp, CONF_SHOWFMT"%.2f\n", "mirrorplotdist", p->mirrorplotdist); if(up->onebinvalueset) fprintf(fp, CONF_SHOWFMT"%.5f\n", "onebinvalue", p->onebinvalue); /* Histogram: */ fprintf(fp, "\n# Histogram:\n"); if(up->histnumbinsset) fprintf(fp, CONF_SHOWFMT"%zu\n", "histnumbins", p->histnumbins); if(up->histminset) fprintf(fp, CONF_SHOWFMT"%.5f\n", "histmin", p->histmin); if(up->histmaxset) fprintf(fp, CONF_SHOWFMT"%.5f\n", "histmax", p->histmax); if(up->histquantset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "histquant", p->histquant); /* Cumulative frequency plot: */ fprintf(fp, "\n# Cumulative frequency plot:\n"); if(up->cfpnumset) fprintf(fp, CONF_SHOWFMT"%zu\n", "cfpnum", p->cfpnum); if(up->cfpminset) fprintf(fp, CONF_SHOWFMT"%.5f\n", "cfpmin", p->cfpmin); if(up->cfpmaxset) fprintf(fp, CONF_SHOWFMT"%.5f\n", "cfpmax", p->cfpmax); if(up->cfpquantset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "cfpquant", p->cfpquant); /* Sigma clipping: */ if(up->sigclipmultipset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "sigclipmultip", p->sigclipmultip); if(up->sigcliptoleranceset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "sigcliptolerance", p->sigcliptolerance); if(up->sigclipnumset) fprintf(fp, CONF_SHOWFMT"%zu\n", "sigclipnum", p->sigclipnum); /* For the operating mode, first put the macro to print the common options, then the (possible options particular to this program). */ fprintf(fp, "\n# Operating mode:\n"); GAL_CONFIGFILES_PRINT_COMMONOPTIONS; } /* Note that numthreads will be used automatically based on the configure time. Note that those options which are not mandatory must not be listed here. */ void checkifset(struct imgstatparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; int intro=0; if(cp->hduset==0) GAL_CONFIGFILES_REPORT_NOTSET("hdu"); if(up->mirrordistset==0) GAL_CONFIGFILES_REPORT_NOTSET("mirrordist"); if(up->mirrorplotdistset==0) GAL_CONFIGFILES_REPORT_NOTSET("mirrorplotdist"); if(up->onebinvalueset==0) GAL_CONFIGFILES_REPORT_NOTSET("onebinvalue"); if(up->histnumbinsset==0) GAL_CONFIGFILES_REPORT_NOTSET("histnumbins"); if(up->cfpnumset==0) GAL_CONFIGFILES_REPORT_NOTSET("cfpnum"); if(up->sigclipmultipset==0) GAL_CONFIGFILES_REPORT_NOTSET("sigclipmultip"); if(up->sigcliptoleranceset==0) GAL_CONFIGFILES_REPORT_NOTSET("sigcliptolerance"); if(up->sigclipnumset==0) GAL_CONFIGFILES_REPORT_NOTSET("sigclipnum"); GAL_CONFIGFILES_END_OF_NOTSET_REPORT; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ void sanitycheck(struct imgstatparams *p) { char *basename; /* Make sure the input file exists. */ gal_checkset_check_file(p->up.inputname); /* Set the p->up.maskname accordingly: */ gal_fits_file_or_ext_name(p->up.inputname, p->cp.hdu, p->up.masknameset, &p->up.maskname, p->up.mhdu, p->up.mhduset, "mask"); /* Set the names of the output files: */ if(p->cp.outputset) basename=p->cp.output; else basename=p->up.inputname; if(p->histname) { p->histname=NULL; /* It wasn't allocated. */ gal_checkset_automatic_output(basename, "_hist.txt", p->cp.removedirinfo, p->cp.dontdelete, &p->histname); } if(p->cfpname) { p->cfpname=NULL; /* It wasn't allocated. */ gal_checkset_automatic_output(basename, "_cfp.txt", p->cp.removedirinfo, p->cp.dontdelete, &p->cfpname); } if(p->mhistname) /* The mode mirror distribution will need */ { /* both a histogram and cfp. */ p->mcfpname=p->mhistname=NULL; gal_checkset_automatic_output(basename, "_modehist.txt", p->cp.removedirinfo, p->cp.dontdelete, &p->mhistname); gal_checkset_automatic_output(basename, "_modecfp.txt", p->cp.removedirinfo, p->cp.dontdelete, &p->mcfpname); } if(isnan(p->mirror)==0) { p->mirrorhist=p->mirrorcfp=NULL; gal_checkset_automatic_output(basename, "_mirrorhist.txt", p->cp.removedirinfo, p->cp.dontdelete, &p->mirrorhist); gal_checkset_automatic_output(basename, "_mirrorcfp.txt", p->cp.removedirinfo, p->cp.dontdelete, &p->mirrorcfp); } /* If the cumulative frequency plot parameters are to depend on the histogram, then make sure that the histogram will be created.*/ if(p->cfpname && p->histname==NULL) { if(p->cfpsimhist) error(EXIT_FAILURE, 0, "without a histogram, `--cfpsimhist` is " "meaningless"); if (p->maxcfpeqmaxhist) error(EXIT_FAILURE, 0, "without a histogram, `--maxcfpeqmaxhist` " "is meaningless"); } /* Check if `--maxcfpeqmaxhist` and `--normcfp` are not called together: */ if(p->normcfp && p->maxcfpeqmaxhist) error(EXIT_FAILURE, 0, "`--normcfp` and `--maxcfpeqmaxhist` " "cannot be called together\n"); /* Check if `normhist` and `maxhistone` are not called together: */ if(p->normhist && p->maxhistone) error(EXIT_FAILURE, 0, "`--normhist` and `--histnumbins` cannot be " "called together\n"); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ void preparearrays(struct imgstatparams *p) { float min; size_t s0, s1; int bitpix, anyblank; struct uiparams *up=&p->up; /* Read the input and mask arrays: */ gal_fits_file_to_float(up->inputname, up->maskname, p->cp.hdu, up->mhdu, &p->img, &bitpix, &anyblank, &s0, &s1); p->size=s0*s1; /* If the minimum value is to be used as a mask then do it: */ if(p->ignoremin) { gal_statistics_float_min(p->img, p->size, &min); gal_array_freplace_value(p->img, p->size, min, NAN); } /* Move all the non-nan elements to the start of the array: */ gal_array_no_nans(p->img, &p->size); /* Make a sorted array for most of the jobs: */ gal_array_float_copy(p->img, p->size, &p->sorted); qsort(p->sorted, p->size, sizeof *p->sorted, gal_qsort_float_increasing); /* Check the given range: */ if(p->histname || p->asciihist || p->mhistname || p->mirrorhist) { if(up->histquantset) { if(p->histquant>=0.5) error(EXIT_FAILURE, 0, "the value to `--histquant' (-Q) must " "Be smaller than 0.5, because it sets the lower limit of " "the value range. The higher limit will be 1-Q"); p->histmin= p->sorted[gal_statistics_index_from_quantile(p->size, p->histquant)]; p->histmax= p->sorted[gal_statistics_index_from_quantile(p->size, 1 - p->histquant)]; } else { switch(up->histminset+up->histmaxset) { case 0: p->histmin=p->sorted[0]; p->histmax=p->sorted[p->size-1]; break; case 1: error(EXIT_FAILURE, 0, "the options `--histmin' (-i) and " "`--histmax' (-x) should both be specified. You have " "only given the %s"GAL_STRINGS_HOW_TO_CHECK_VALUES, up->histminset==1 ? "former" : "latter"); break; case 2: if(p->histmin>=p->histmax) error(EXIT_FAILURE, 0, "the value to `--histmin' (-i) (%f) " "is larger or equal to that of `--histmax' (-x) (%f)" GAL_STRINGS_HOW_TO_CHECK_VALUES, p->histmin, p->histmax); if(p->histmin>p->sorted[p->size-1] || p->histmaxsorted[0]) error(EXIT_FAILURE, 0, "the range of data is %.5f to %.5f. " "However, you have set `--histmin' (-i) and " "`--histmax' (-x) to %.5f and %.5f respectively. " "They do not overlap"GAL_STRINGS_HOW_TO_CHECK_VALUES, p->sorted[0], p->sorted[p->size-1], p->histmin, p->histmax); break; default: error(EXIT_FAILURE, 0, "a bug! Please contact us at " PACKAGE_BUGREPORT" So we can solve the problem. the " "value of up->histminset+up->histmaxset is not 0, 1 or " "2"); } } } else /* For the ascii histogram. */ { p->histmin=p->sorted[0]; p->histmax=p->sorted[p->size-1]; } if(p->cfpname && p->cfpsimhist==0) { if(up->cfpquantset) { if(p->cfpquant>=0.5) error(EXIT_FAILURE, 0, "the value to `--cfpquant' (-U) must " "Be smaller than 0.5, because it sets the lower limit of " "the value range. The higher limit will be 1-U"); p->cfpmin=p->sorted[gal_statistics_index_from_quantile(p->size, p->cfpquant)]; p->cfpmax= p->sorted[gal_statistics_index_from_quantile(p->size, 1 - p->cfpquant)]; } else { switch(up->cfpminset+up->cfpmaxset) { case 0: p->cfpmin=p->sorted[0]; p->cfpmax=p->sorted[p->size-1]; break; case 1: error(EXIT_FAILURE, 0, "the options `--cfpmin' (-a) and " "`--cfpmax' (-b) should both be specified. You have " "only given the %s"GAL_STRINGS_HOW_TO_CHECK_VALUES, up->cfpminset==1 ? "former" : "latter"); break; case 2: if(p->cfpmin>p->cfpmax) error(EXIT_FAILURE, 0, "the value to `--cfpmin' (-a) (%.f) " "is larger than that of `--cfpmax' (-b) (%f)" GAL_STRINGS_HOW_TO_CHECK_VALUES, p->cfpmin, p->cfpmax); if(p->cfpmin>p->sorted[p->size-1] || p->cfpmaxsorted[0]) error(EXIT_FAILURE, 0, "the range of data is %.5f to %.5f. " "However, you have set `--cfpmin' (-a) and " "`--cfpmax' (-b) to %.5f and %.5f respectively. " "They do not overlap"GAL_STRINGS_HOW_TO_CHECK_VALUES, p->sorted[0], p->sorted[p->size-1], p->cfpmin, p->cfpmax); break; default: error(EXIT_FAILURE, 0, "a bug! Please contact us at " PACKAGE_BUGREPORT" So we can solve the problem. the " "value of up->cfpminset+up->cfpmaxset is not 0, 1 or " "2"); } } } } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void setparams(int argc, char *argv[], struct imgstatparams *p) { struct gal_commonparams *cp=&p->cp; /* Set the non-zero initial values, the structure was initialized to have a zero value for all elements. */ cp->spack = SPACK; cp->verb = 1; cp->numthreads = num_processors(NPROC_CURRENT); cp->removedirinfo = 1; p->asciihist = 1; p->sigclip = 1; p->mirror = NAN; p->onebinvalue = NAN; p->histname=p->cfpname="a"; /* Will be set later, just a sign that */ /* they should be output. */ /* Read the arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Add the user default values and save them if asked. */ GAL_CONFIGFILES_CHECK_SET_CONFIG; /* Check if all the required parameters are set. */ checkifset(p); /* Print the values for each parameter. */ if(cp->printparams) GAL_CONFIGFILES_REPORT_PARAMETERS_SET; /* Do a sanity check. */ sanitycheck(p); /* Make the array of input images. */ preparearrays(p); /* Everything is ready, notify the user of the program starting. */ if(cp->verb) { printf(SPACK_NAME" started on %s", ctime(&p->rawtime)); printf(" - Input read: %s (hdu: %s)\n", p->up.inputname, p->cp.hdu); if(p->up.maskname) printf(" - Mask read: %s (hdu: %s)\n", p->up.maskname, p->up.mhdu); } } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void freeandreport(struct imgstatparams *p, struct timeval *t1) { /* Free the allocated arrays: */ free(p->img); free(p->sorted); free(p->cp.hdu); free(p->cfpname); free(p->histname); free(p->mcfpname); free(p->mhistname); free(p->cp.output); if(p->up.masknameallocated) free(p->up.maskname); /* Print the final message. */ if(p->cp.verb) gal_timing_report(t1, SPACK_NAME" finished in: ", 0); } gnuastro-0.2.33-8a3b/bin/imgstat/cite.h0000644000175000017500000000320112750745735014445 00000000000000/********************************************************************* ImageStatistics - Get general statistics about the image. ImgeStatistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CITE_H #define CITE_H #define IMGSTATBIBTEX "" #define PRINTCITEABORT { \ printf("\nWe hope %s has been useful for your research.\n" \ "Citations are vital for the continued work on %s.\n" \ "Thank you for citing it in your research paper.\n" \ "\nPlease cite as \"%s\":\n\n%s\n\n%s", \ SPACK_NAME, SPACK_NAME, SPACK_STRING, \ GAL_STRINGS_MAIN_BIBTEX, IMGSTATBIBTEX); \ exit(EXIT_SUCCESS); \ } #endif gnuastro-0.2.33-8a3b/bin/imgstat/main.h0000644000175000017500000001242413001632537014435 00000000000000/********************************************************************* ImageStatistics - Get general statistics about the image. ImgeStatistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include /* Progarm name macros: */ #define SPACK "astimgstat" /* Subpackage executable name. */ #define SPACK_NAME "ImageStatistics" /* Subpackage full name. */ #define SPACK_STRING SPACK_NAME" ("PACKAGE_NAME") "PACKAGE_VERSION #define PRINTFLT "%.6f\n" #define PRINTINT "%.0f\n" #define STRVAL " -- %-45s%s\n" #define FNAMEVAL " -- %-45s%f\n" #define SNAMEVAL " -- %-45s%zu\n" #define ASCIIHISTNUMBINS 60 #define ASCIIHISTHEIGHT 10 #define HISTSTRING "Histogram" #define CFPSTRING "Cumulative Frequency Plot" struct uiparams { char *inputname; /* Name of input file. */ char *maskname; /* Name of mask image. */ char *mhdu; /* Mask image HDU. */ int masknameset; int masknameallocated; int mhduset; int mirrordistset; int onebinvalueset; int histnumbinsset; int histminset; int histmaxset; int histquantset; int cfpnumset; int cfpminset; int cfpmaxset; int cfpquantset; int mirrorplotdistset; int sigclipmultipset; int sigcliptoleranceset; int sigclipnumset; }; struct imgstatparams { /* Other structures: */ struct uiparams up; /* User interface parameters. */ struct gal_commonparams cp; /* Common parameters. */ /* Input: */ float *img; /* Input image array. */ float *sorted; /* Sorted input data. */ size_t size; /* Number of non-blank data elements. */ int ignoremin; /* Ignore all data with minimum value. */ float mirrordist; /* Distance to go out for mode check. */ /* Output: */ int asciihist; /* ==1: print an ASCII histogram. */ float onebinvalue; /* Shift bins so one bin starts with this. */ int lowerbin; /* Interval lower limit as column 1. */ float mirror; /* Mirror quantile. */ char *mirrorhist; /* Name of mirror histogram. */ char *mirrorcfp; /* Name of mirror CFP. */ char *mhistname; /* Name of mode mirror histogram. */ float mirrorplotdist; /* Dist. after mode to display on plot. */ char *mcfpname; /* Name of mode mirror CFP. */ int histrangeformirror; /* ==1: Use histogram range for mirror. */ /* Histogram: */ char *histname; /* Histogram file name. */ int normhist; /* ==1: Normalize the histogram. */ int maxhistone; /* Scale such that max bin is one. */ size_t histnumbins; /* Number of bins in the histogram. */ float histmin; /* Minimum value to use in histogram. */ float histmax; /* Maximum value to use in histogram. */ float histquant; /* Quantile range of histogram. */ /* Cumulative frequency plot: */ char *cfpname; /* Cumultiave frequency plot file name. */ int normcfp; /* ==1: Normalize the CFP. */ int maxcfpeqmaxhist; /* ==1: CFP max equal to historgram max. */ int cfpsimhist; /* ==1: CFP range equal to hist range. */ size_t cfpnum; /* The number of points to sample CFP. */ float cfpmin; /* Minimum value for CFP. */ float cfpmax; /* Maximum value for CFP. */ float cfpquant; /* Quantile range of CFP. */ /* Sigma clipping: */ int sigclip; /* ==1: Do sigma clipping. */ float sigclipmultip; /* Multiple of STD in sigma clipping. */ float sigcliptolerance; /* Tolerance level in sigma clipping. */ size_t sigclipnum; /* Number of times to sigma clip. */ /* Operating mode: */ /* Internal: */ time_t rawtime; /* Starting time of the program. */ }; #endif gnuastro-0.2.33-8a3b/bin/imgstat/main.c0000644000175000017500000000322712774156725014451 00000000000000/********************************************************************* ImageStatistics - Get general statistics about the image. ImgeStatistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include /* Includes time.h and sys/time.h */ #include "main.h" #include "ui.h" /* needs main.h. */ #include "imgstat.h" /* needs main.h. */ int main (int argc, char *argv[]) { struct timeval t1; struct imgstatparams p={{0}, {0}, 0}; /* Set the starting time. */ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ setparams(argc, argv, &p); /* Run MakeProfiles */ imgstat(&p); /* Free all non-freed allocations. */ freeandreport(&p, &t1); /* Return successfully.*/ return 0; } gnuastro-0.2.33-8a3b/bin/imgstat/Makefile.in0000644000175000017500000017251713004464626015424 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or 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= @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ 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.NOEXPORT: gnuastro-0.2.33-8a3b/bin/imgstat/astimgstat.conf0000644000175000017500000000176112575241010016366 00000000000000# Default parameters (System) for ImageStatistics. # ImageStatistics is part of GNU Astronomy Utitlies. # # Use the long option name of each paramter followed by # a value. The name and value should be separated by # atleast one of the following charaacters: # space, `,`, `=` or `:` # # Run with `--help` option or read the manual for a full # explanation of what each option means. # # NOTE I: All counting is from zero, not one. # NOTE II: Lines starting with `#` are ignored. # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Input image: hdu 0 mirrordist 1.5 # Output: mirrorplotdist 2 onebinvalue nan # Histogram: histnumbins 200 # Cumulative frequency plot: cfpnum 200 sigclipmultip 4.000 sigcliptolerance 0.200 sigclipnum 5gnuastro-0.2.33-8a3b/bin/imgstat/Makefile.am0000644000175000017500000000270012765246731015405 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. NOTE: $(top_srcdir)/bootstrapped/lib is only necessary ## for internally compiled utilities and libraries. It must not be included ## during the tests since the bootstrapped libraries are not installed. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Utility and its sources bin_PROGRAMS = astimgstat astimgstat_SOURCES = main.c main.h cite.h ui.c ui.h args.h \ imgstat.c imgstat.h astimgstat_LDADD = $(top_builddir)/bootstrapped/lib/libgnu.la \ -lgnuastro ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astimgstat.conf gnuastro-0.2.33-8a3b/bin/imgcrop/0000755000175000017500000000000013004464724013411 500000000000000gnuastro-0.2.33-8a3b/bin/imgcrop/crop.h0000644000175000017500000000513312764767045014465 00000000000000/********************************************************************* ImageCrop - Crop a given size from one or multiple images. ImageCrop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CROP_H #define CROP_H #include #include struct cropparams { void *array; /* Pointer to basic structure: */ struct imgcropparams *p; /* About input image. */ size_t imgindex; /* Index of this image in the input names. */ fitsfile *infits; /* Pointer to the input FITS image. */ long fpixel[2]; /* Position of first pixel in input image. */ long lpixel[2]; /* Position of last pixel in input image. */ double *ipolygon; /* Input image based polygon vertices. */ /* Output (cropped) image. */ double world[2]; /* World coordinates of crop center. */ double sized[2]; /* Width and height of image in degrees. */ double corners[8]; /* RA and Dec of this crop's four sides. */ double equatorcorr[2]; /* Crop crosses the equator, see wcsmode.c. */ size_t outlen; /* Length of output name. */ size_t outindex; /* Index of this crop in the output list. */ fitsfile *outfits; /* Pointer to the output FITS image. */ /* Thread parameters. */ size_t *indexs; /* Indexs to be used in this thread. */ pthread_barrier_t *b; /* pthread barrier to keep threads waiting. */ }; void polygonparser(struct imgcropparams *p); void sectionparser(char *section, long *naxes, long *fpixel, long *lpixel); void cropname(struct cropparams *crp); void cropflpixel(struct cropparams *crp); void onecrop(struct cropparams *crp); int iscenterfilled(struct cropparams *crp); void printlog(struct imgcropparams *p); #endif gnuastro-0.2.33-8a3b/bin/imgcrop/crop.c0000644000175000017500000006774613001632537014460 00000000000000/********************************************************************* ImageCrop - Crop a given size from one or multiple images. ImageCrop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include "main.h" #include "crop.h" #include "wcsmode.h" /*******************************************************************/ /************ Set/correct first and last pixel **************/ /*******************************************************************/ /* Read the section string and set the starting and ending pixels based on that. */ void sectionparser(char *section, long *naxes, long *fpixel, long *lpixel) { int add; long read; size_t dim=0; char *tailptr; char forl='f', *pt=section; /* Initialize the fpixel and lpixel arrays: */ lpixel[0]=naxes[0]; lpixel[1]=naxes[1]; fpixel[0]=fpixel[1]=1; /* Parse the string. */ while(*pt!='\0') { add=0; switch(*pt) { case ',': ++dim; if(dim==2) error(EXIT_FAILURE, 0, "Extra `,` in `%s`", section); forl='f'; ++pt; break; case ':': forl='l'; ++pt; break; case '.': error(EXIT_FAILURE, 0, "the numbers in the argument to " "`--section` (`-s') have to be integers. You input " "includes a float number: %s", section); break; case ' ': case '\t': ++pt; break; case '*': add=1; /* If it is an asterisk, then add the */ ++pt; /* given value to the maximum size of */ break; /* the image. */ default: break; } /* Read the number: */ read=strtol(pt, &tailptr, 0); /* Check if there actually was a number. printf("\n\n------\n%c: %ld (%s)\n", *pt, read, tailptr); */ /* Make sure if a number was read at all? */ if(tailptr==pt) /* No number was read! */ { if(add) read=0; /* We have a * followed by `:' or `,'. */ else continue; } /* Put it in the correct array. Note that for the last point, we don't want to include the given pixel. Unlike CFITSIO, in ImageCrop, the given intervals are not inclusive. fpixel and lpixel will be directly passed to CFITSIO. So we have to correct his here.*/ if(forl=='f') fpixel[dim] = add ? naxes[dim]+read : read; else lpixel[dim] = add ? naxes[dim]+read-1 : read-1; pt=tailptr; /* For a check: printf("\n\n[%ld, %ld]: fpixel=(%ld, %ld), lpixel=(%ld, %ld)\n\n", naxes[0], naxes[1], fpixel[0], fpixel[1], lpixel[0], lpixel[1]); */ } if(fpixel[0]>=lpixel[0] || fpixel[1]>=lpixel[1]) error(EXIT_FAILURE, 0, "the bottom left corner coordinates " "cannot be larger or equal to the top right's! Your section " "string (%s) has been read as: bottom left coordinate " "(%ld, %ld) to top right coordinate (%ld, %ld)", section, fpixel[0], fpixel[1], lpixel[0], lpixel[1]); /* printf("\n%s\nfpixel=(%ld, %ld), lpixel=(%ld, %ld)\n\n", section, fpixel[0], fpixel[1], lpixel[0], lpixel[1]); exit(0); */ } void polygonparser(struct imgcropparams *p) { size_t dim=0; char *tailptr; double read[2], *array; struct gal_linkedlist_tdll *gal_linkedlist_tdll=NULL; char *pt=p->up.polygon; /* Parse the string. */ while(*pt!='\0') { switch(*pt) { case ',': ++dim; if(dim==2) error(EXIT_FAILURE, 0, "Extra `,` in `%s`", p->up.polygon); ++pt; break; case ':': if(dim==0) error(EXIT_FAILURE, 0, "not enough coordinates for at least " "one polygon vertex (in %s)", p->up.polygon); dim=0; ++pt; break; default: break; } /* strtod will skip white spaces if they are before a number, but not when they are before a : or ,. So we need to remove all white spaces. White spaces are usually put beside each other, so if one is encountered, go along the string until the white space characters finish. */ if(isspace(*pt)) ++pt; else { /* Read the number: */ read[dim]=strtod(pt, &tailptr); /* Check if there actually was a number. printf("\n\n------\n%zu: %f (%s)\n", dim, read[dim], tailptr); */ /* Make sure if a number was read at all? */ if(tailptr==pt) /* No number was read! */ error(EXIT_FAILURE, 0, "%s could not be parsed as a floating " "point number", tailptr); /* If this was the second dimension, then put the values into the linked list: */ if(dim==1) gal_linkedlist_add_to_tdll(&gal_linkedlist_tdll, read[0], read[1]); /* The job here is done, start from tailptr */ pt=tailptr; } } /* Convert the linked list to an array: */ gal_linkedlist_tdll_to_array_inv(gal_linkedlist_tdll, &array, &p->nvertices); if(p->imgmode) { p->ipolygon=array; p->wpolygon=NULL; } else { p->ipolygon=NULL; p->wpolygon=array; } /* Put them in the proper order in WCS mode: */ /* For a check: { size_t i; double *polygon=p->imgmode?p->ipolygon:p->wpolygon; for(i=0;invertices;++i) printf("(%f, %f)\n", polygon[i*2], polygon[i*2+1]); } */ /* Clean up: */ gal_linkedlist_free_tdll(gal_linkedlist_tdll); } void imgpolygonflpixel(double *ipolygon, size_t nvertices, long *fpixel, long *lpixel) { size_t i; double minx=FLT_MAX, miny=FLT_MAX; double maxx=-FLT_MAX, maxy=-FLT_MAX; /* Find their minimum and maximum values. */ for(i=0;imaxx) maxx=ipolygon[i*2]; if(ipolygon[i*2]maxy) maxy=ipolygon[i*2+1]; if(ipolygon[i*2+1]=0.5 ? (int)minx + 1 : (int)minx; fpixel[1] = miny - (int)miny >=0.5 ? (int)miny + 1 : (int)miny; lpixel[0] = maxx - (int)maxx >=0.5 ? (int)maxx + 1 : (int)maxx; lpixel[1] = maxy - (int)maxy >=0.5 ? (int)maxy + 1 : (int)maxy; } void polygonmask(struct cropparams *crp, void *array, long *fpixel_i, size_t s0, size_t s1) { long *lb, *la=array; short *sb, *sa=array; float *fb, *fa=array; LONGLONG *Lb, *La=array; unsigned char *bb, *ba=array; double *db, *ipolygon, point[2], *da=array; size_t i, *ordinds, size=s0*s1, nvertices=crp->p->nvertices; int outpolygon=crp->p->outpolygon, datatype=crp->p->datatype; /* First of all, allocate enough space to put a copy of the input coordinates (we will be using that after sorting in an anti-clickwise manner.) */ errno=0; ipolygon=malloc(2*nvertices*sizeof *ipolygon); if(ipolygon==NULL) error(EXIT_FAILURE, errno, "%zu bytes for ipolygon in polygonmask " "(crop.c)", 2*nvertices*sizeof *ipolygon); errno=0; ordinds=malloc(nvertices*sizeof *ordinds); if(ordinds==NULL) error(EXIT_FAILURE, errno, "%zu bytes for ordinds in polygonmask " "(crop.c)", nvertices*sizeof *ordinds); /* Find the order of the polygons and put the elements in the proper order. Also subtract the fpixel_i coordinates from all the vertices to bring them into the crop image coordinates.*/ gal_polygon_ordered_corners(crp->ipolygon, crp->p->nvertices, ordinds); for(i=0;ip->nvertices;++i) { ipolygon[i*2 ] = crp->ipolygon[ordinds[i]*2] - fpixel_i[0]; ipolygon[i*2+1] = crp->ipolygon[ordinds[i]*2+1] - fpixel_i[1]; } /* Go over all the pixels in the image and if they are within the polygon keep them if the user has asked for it.*/ switch(datatype) { case TBYTE: bb=gal_fits_datatype_blank(datatype); for(i=0;ip; struct gal_commonparams *cp=&p->cp; struct imgcroplog *log=&crp->p->log[crp->outindex]; /* Set the output name and crop sides: */ if(p->up.catset) { errno=0; log->name=malloc(crp->outlen); if(log->name==NULL) error(EXIT_FAILURE, errno, "imgmode.c, %zu bytes on " "imgcroponthreads", crp->outlen); sprintf(log->name, "%s%zu%s", cp->output, crp->outindex+1, p->suffix); gal_checkset_check_remove_file(log->name, cp->dontdelete); } else { /* Set the output name. */ if(p->outnameisfile) /* An output file was specified. */ { log->name=cp->output; gal_checkset_check_remove_file(log->name, cp->dontdelete); } else /* The output was a directory, use automatic output. */ gal_checkset_automatic_output(p->imgs[crp->imgindex].name, p->suffix, cp->removedirinfo, cp->dontdelete, &log->name); } } /* Find the first and last pixel of a crop from its center point (in image mode or WCS mode). */ void cropflpixel(struct cropparams *crp) { int ncoord=1, nelem=2, status; struct imgcropparams *p=crp->p; long *naxes=p->imgs[crp->imgindex].naxes; double pixcrd[2], imgcrd[2], phi[1], theta[1]; long *fpixel=crp->fpixel, *lpixel=crp->lpixel; if(p->imgmode) { if(p->up.catset) gal_box_border_from_center(p->cat[crp->outindex*p->cs1+p->xcol], p->cat[crp->outindex*p->cs1+p->ycol], p->iwidth, fpixel, lpixel); else if(p->up.xcset) gal_box_border_from_center(p->xc, p->yc, p->iwidth, fpixel, lpixel); else if(p->up.sectionset) sectionparser(p->section, naxes, fpixel, lpixel); else if(p->up.polygonset) { if(p->outpolygon==0) imgpolygonflpixel(p->ipolygon, p->nvertices, fpixel, lpixel); } else error(EXIT_FAILURE, 0, "a bug! In image mode, neither of the " "following has been set: a catalog, a central pixel, " "a section or a polygon in the image. Please contact us " "to see how it got to this impossible place! You should " "have been warned of this condition long before ImageCrop " "reaches this point"); } else if(p->wcsmode) /* In wcsmode, crp->world is already filled. */ { /* Note that p->iwidth was set based on p->wwidth. */ if(p->up.polygonset) { /* Fill crp->ipolygon in wcspolygonpixel, then set flpixel*/ fillcrpipolygon(crp); if(p->outpolygon==0) imgpolygonflpixel(crp->ipolygon, p->nvertices, fpixel, lpixel); } else { status=0; if(wcss2p(p->imgs[crp->imgindex].wcs, ncoord, nelem, crp->world, phi, theta, imgcrd, pixcrd, &status) ) error(EXIT_FAILURE, 0, "wcss2p error %d: %s", status, wcs_errmsg[status]); gal_box_border_from_center(pixcrd[0], pixcrd[1], p->iwidth, fpixel, lpixel); /* printf("\n(%f, %f): (%ld, %ld) -- (%ld, %ld)\n\n", pixcrd[0], pixcrd[1], fpixel[0], fpixel[1], lpixel[0], lpixel[1]); */ } } else error(EXIT_FAILURE, 0, "a bug! in cropflpixel (crop.c), " "neither imgmode or wcsmode are set. Please contact us so " "we can see how it got to this impossible place"); /* If the user only wants regions outside to the polygon, then set the fpixel and lpixel to cover the full input image. */ if(p->up.polygonset && p->outpolygon) { crp->lpixel[0]=naxes[0]; crp->lpixel[1]=naxes[1]; crp->fpixel[0]=crp->fpixel[1]=1; } } /* Find the size of the final FITS image (irrespective of how many crops will be needed for it) and make the image to keep the data. NOTE: The fpixel and lpixel in crp keep the first and last pixel of the total image for this crop, irrespective of the final keeping blank areas or not. While the fpixel_i and lpixel_i arrays keep the first and last pixels after the blank pixels have been removed. */ void firstcropmakearray(struct cropparams *crp, long *fpixel_i, long *lpixel_i, long *fpixel_c, long *lpixel_c) { size_t i; fitsfile *ofp; long naxes[2]; double crpix0, crpix1; int naxis=2, status=0; int bitpix=crp->p->bitpix; char *cp, *cpf, blankrec[80], titlerec[80]; char startblank[]=" / "; char *outname=crp->p->log[crp->outindex].name; struct inputimgs *img=&crp->p->imgs[crp->imgindex]; /* Set the last element of the blank array. */ cpf=blankrec+79; *cpf='\0'; titlerec[79]='\0'; cp=blankrec; do *cp=' '; while(++cpp->noblank && crp->p->wcsmode==0) { fpixel_c[0]=fpixel_c[1]=1; lpixel_c[0]=naxes[0]=lpixel_i[0]-fpixel_i[0]+1; lpixel_c[1]=naxes[1]=lpixel_i[1]-fpixel_i[1]+1; } else { naxes[0]=crp->lpixel[0]-crp->fpixel[0]+1; naxes[1]=crp->lpixel[1]-crp->fpixel[1]+1; } /* Create the FITS image extension and array and fill it with null values. */ if(fits_create_file(&crp->outfits, outname, &status)) gal_fits_io_error(status, "creating file"); ofp=crp->outfits; if(fits_create_img(ofp, bitpix, naxis, naxes, &status)) gal_fits_io_error(status, "creating image"); if(bitpix==BYTE_IMG || bitpix==SHORT_IMG || bitpix==LONG_IMG || bitpix==LONGLONG_IMG) if(fits_write_key(ofp, crp->p->datatype, "BLANK", crp->p->bitnul, "pixels with no data", &status) ) gal_fits_io_error(status, "adding Blank"); if(fits_write_null_img(ofp, 1, naxes[0]*naxes[1], &status)) gal_fits_io_error(status, "writing null array"); /* Write the WCS header keywords in the output FITS image, then update the header keywords. */ if(img->wcs) { crpix0 = img->wcs->crpix[0] - (fpixel_i[0]-1) + (fpixel_c[0]-1); crpix1 = img->wcs->crpix[1] - (fpixel_i[1]-1) + (fpixel_c[1]-1); if(fits_write_record(ofp, blankrec, &status)) gal_fits_io_error(status, NULL); sprintf(titlerec, "%sWCS information", startblank); for(i=strlen(titlerec);i<79;++i) titlerec[i]=' '; fits_write_record(ofp, titlerec, &status); for(i=0;inwcskeys-1;++i) fits_write_record(ofp, &img->wcstxt[i*80], &status); fits_update_key(ofp, TDOUBLE, "CRPIX1", &crpix0, NULL, &status); fits_update_key(ofp, TDOUBLE, "CRPIX2", &crpix1, NULL, &status); gal_fits_io_error(status, NULL); } /* Add the Crop information. */ if(fits_write_record(ofp, blankrec, &status)) gal_fits_io_error(status, NULL); sprintf(titlerec, "%sCrop information", startblank); for(i=strlen(titlerec);i<79;++i) titlerec[i]=' '; if(fits_write_record(ofp, titlerec, &status)) gal_fits_io_error(status, NULL); } /* The starting and ending points are set in the cropparams structure for one crop from one image. Crop that region out. return values are: 0: No crop was made (not in range of image). 1: The input image covered at least part of the crop image. */ void onecrop(struct cropparams *crp) { struct imgcropparams *p=crp->p; struct inputimgs *img=&p->imgs[crp->imgindex]; void *array; size_t cropsize; char basename[FLEN_KEYWORD]; long fpixel_i[2] , lpixel_i[2]; fitsfile *ifp=crp->infits, *ofp; struct gal_fits_key_ll *headers=NULL; int status=0, anynul=0, bitpix=p->bitpix; long fpixel_o[2], lpixel_o[2], inc[2]={1,1}; char region[FLEN_VALUE], regionkey[FLEN_KEYWORD]; /* Find the first and last pixel of this crop box from this input image. If the outer polygon region is to be kept, then set the sides to the image sides.*/ cropflpixel(crp); fpixel_i[0]=crp->fpixel[0]; fpixel_i[1]=crp->fpixel[1]; lpixel_i[0]=crp->lpixel[0]; lpixel_i[1]=crp->lpixel[1]; /* Find the overlap and apply it if there is any overlap. */ if( gal_box_overlap(img->naxes, fpixel_i, lpixel_i, fpixel_o, lpixel_o) ) { /* Make the output FITS image and initialize it with an array of NaN or BLANK values. Note that for FLOAT_IMG and DOUBLE_IMG, it will automatically fill them with the NaN value.*/ if(crp->outfits==NULL) firstcropmakearray(crp, fpixel_i, lpixel_i, fpixel_o, lpixel_o); ofp=crp->outfits; /* Read the desired part of the image, then write it into this array. */ cropsize=(lpixel_i[0]-fpixel_i[0]+1)*(lpixel_i[1]-fpixel_i[1]+1); array=gal_fits_datatype_alloc(cropsize, p->datatype); status=0; if(fits_read_subset(ifp, p->datatype, fpixel_i, lpixel_i, inc, p->bitnul, array, &anynul, &status)) gal_fits_io_error(status, NULL); /* If we have a floating point or double image, pixels with zero value should actually be a NaN. Unless the user specificly asks for it, make the conversion.*/ if(p->zeroisnotblank==0 && (bitpix==FLOAT_IMG || bitpix==DOUBLE_IMG) ) changezerotonan(array, cropsize, bitpix); /* If a polygon is given, remove all the pixels within or outside of it.*/ if(p->up.polygonset) { /* In WCS mode, crp->ipolygon was allocated and filled in wcspolygonflpixel (wcsmode.c). */ if(p->imgmode) crp->ipolygon=p->ipolygon; polygonmask(crp, array, fpixel_i, lpixel_i[1]-fpixel_i[1]+1, lpixel_i[0]-fpixel_i[0]+1); if(p->wcsmode) free(crp->ipolygon); } /* Write the array into the image. */ status=0; if( fits_write_subset(ofp, p->datatype, fpixel_o, lpixel_o, array, &status) ) gal_fits_io_error(status, NULL); /* A section has been added to the cropped image from this input image, so increment crp->imgcount and save the information of this image. */ sprintf(basename, "ICF%zu", ++p->log[crp->outindex].numimg); gal_fits_file_name_in_keywords(basename, img->name, &headers); sprintf(regionkey, "%sPIX", basename); sprintf(region, "%ld:%ld,%ld:%ld", fpixel_i[0], lpixel_i[0]+1, fpixel_i[1], lpixel_i[1]+1); gal_fits_add_to_key_ll_end(&headers, TSTRING, regionkey, 0, region, 0, "Range of pixels used for this output.", 0, NULL); gal_fits_update_keys(ofp, &headers); /* Free the allocated array. */ free(array); } else if(p->up.polygonset && p->outpolygon==0 && p->wcsmode) free(crp->ipolygon); return; } /*******************************************************************/ /****************** Check center *********************/ /*******************************************************************/ int iscenterfilled(struct cropparams *crp) { struct imgcropparams *p=crp->p; void *array; int bitpix=p->bitpix; size_t size, nulcount; fitsfile *ofp=crp->outfits; int status=0, maxdim=10, anynul; long checkcenter=p->checkcenter; long naxes[2], fpixel[2], lpixel[2], inc[2]={1,1}; uint8_t *b, *fb, *nb; int16_t *s, *fs, *ns; int32_t *l, *fl, *nl; int64_t *L, *fL, *nL; float *f, *ff; /* isnan will check. */ double *d, *fd; /* isnan will check */ /* Get the final size of the output image. */ if( fits_get_img_size(ofp, maxdim, naxes, &status) ) gal_fits_io_error(status, NULL); /* Get the size and range of the central region to check. The +1 is because in FITS, counting begins from 1, not zero. */ fpixel[0]=(naxes[0]/2+1)-checkcenter/2; fpixel[1]=(naxes[1]/2+1)-checkcenter/2; lpixel[0]=(naxes[0]/2+1)+checkcenter/2; lpixel[1]=(naxes[1]/2+1)+checkcenter/2; /* Allocate the array and read in the pixels. */ size=checkcenter*checkcenter; array=gal_fits_datatype_alloc(size, gal_fits_bitpix_to_datatype(bitpix) ); if( fits_read_subset(ofp, p->datatype, fpixel, lpixel, inc, p->bitnul, array, &anynul, &status) ) gal_fits_io_error(status, NULL); /* Depending on bitpix, check the central pixels of the image. */ nulcount=0; switch(bitpix) { case BYTE_IMG: nb=p->bitnul; fb=(b=array)+size; do if(*b==*nb) ++nulcount; while(++bbitnul; fs=(s=array)+size; do if(*s==*ns) ++nulcount; while(++sbitnul; fl=(l=array)+size; do if(*l==*nl) ++nulcount; while(++lbitnul; fL=(L=array)+size; do if(*L==*nL) ++nulcount; while(++Llog; size_t numfiles=0, numcentfilled=0, numstitched=0; /* Only for a catalog are these statistics worth it! */ if(p->up.catset && p->cp.verb) for(i=0;log[i].name;++i) if(log[i].numimg) { if(log[i].centerfilled || p->keepblankcenter) { ++numfiles; if(log[i].numimg>1) ++numstitched; } if(log[i].centerfilled) ++numcentfilled; } /* Check to see if the file exists and remove if if it is ok. */ gal_checkset_check_remove_file(LOGFILENAME, p->cp.dontdelete); /* Make the file and print the top comments. If the file can't be opened for write mode, there is no problem, this is a log file, the user can set it on verbose mode and the same information will be printed. */ errno=0; logfile=fopen(LOGFILENAME, "w"); if(logfile) { /* First print the comments to the file. */ fprintf(logfile, "# "SPACK_STRING" log file.\n" "# "SPACK_NAME" was run on %s#\n", ctime(&p->rawtime)); if(p->keepblankcenter==0) fprintf(logfile, "# NOTE: by default images with a blank " "center are deleted.\n# To keep such images, run again " "with `--keepblankcenter`.\n#\n"); fprintf(logfile, "# Column numbers below start from zero.\n" "# 0: Output file name.\n" "# 1: Number of images used in this cropped image.\n" "# 2: Are the central %zu pixels filled? (1: yes, 0: no)\n", p->checkcenter); /* Then print each output's information. */ for(i=0;log[i].name;++i) fprintf(logfile, "%s %-8zu%-2d\n", log[i].name, log[i].numimg, log[i].centerfilled); /* Report Summary: */ if(p->cp.verb && p->up.catset) { sprintf(msg, "%zu images created.", numfiles); gal_timing_report(NULL, msg, 1); sprintf(msg, "%zu filled in the center.", numcentfilled); gal_timing_report(NULL, msg, 1); if(numstitched) { sprintf(msg, "%zu used more than one input.", numstitched); gal_timing_report(NULL, msg, 1); } } /* Close the file. */ errno=0; if(fclose(logfile)) error(EXIT_FAILURE, errno, LOGFILENAME" could not be closed"); } } gnuastro-0.2.33-8a3b/bin/imgcrop/wcsmode.h0000644000175000017500000000234012616616510015142 00000000000000/********************************************************************* ImageCrop - Crop a given size from one or multiple images. ImageCrop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef WCSMODE_H #define WCSMODE_H void wcscheckprepare(struct imgcropparams *p, struct inputimgs *img); void setcsides(struct cropparams *crp); void fillcrpipolygon(struct cropparams *crp); int radecoverlap(struct cropparams *crp); #endif gnuastro-0.2.33-8a3b/bin/imgcrop/wcsmode.c0000644000175000017500000004041013001632537015131 00000000000000/********************************************************************* ImageCrop - Crop a given size from one or multiple images. ImageCrop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include "main.h" #include "crop.h" /*******************************************************************/ /**************** Check for ui.c *********************/ /*******************************************************************/ /* This function is called from ui.c. Its job is to check the WCS values of this */ void wcscheckprepare(struct imgcropparams *p, struct inputimgs *img) { double twidth; struct wcsprm *wcs=img->wcs; int status, ncoord=4, nelem=2; double imgcrd[8], phi[4], theta[4], pixcrd[8]; /* Check if the image is aligned correctly and fits the resolution of other images. */ if(wcs->pc[1]!=0.0f || wcs->pc[2]!=0.0f) error(EXIT_FAILURE, 0, "%s: HDU %s: is not aligned to the " "celestial coordinates. The first FITS axis should be " "along the Right Ascension and the second FITS axis " "should be along the declination. You should rotate " "(interpolate) the images with other software", img->name, p->cp.hdu); if(wcs->pc[0]>0) error(EXIT_FAILURE, 0, "%s: HDU %s: An increase in the first " "FITS axis pixel coordinates should be a decrese in the " "RA. You have to flip the image along the second axis " "before running ImageCrop", img->name, p->cp.hdu); if(wcs->pc[3]<0) error(EXIT_FAILURE, 0, "%s: HDU %s: An increase in the second " "FITS axis pixel coordinates should translate to an " "increase in the declination. You have to flip the " "image along the first axis before running ImageCrop", img->name, p->cp.hdu); /* Since we are dealing with very accurate values, a multiplication by -1 might cause a floating point error. So we have to account for the floating point error. */ if(-1.0f*wcs->pc[0]pc[3]-1e-15 || -1.0f*wcs->pc[0]>wcs->pc[3]+1e-15) error(EXIT_FAILURE, 0, "%s: HDU %s: The pixel scale along " "the two image axises is not the same. The first axis " "is %f arcseconds/pixel, while the second is %f", img->name, p->cp.hdu, 3600*-1.0f*wcs->pc[0], 3600*wcs->pc[3]); if(p->res==0.0f) { /* Set the resolution of the image. */ p->res=wcs->pc[3]; /* Set the widths such that iwidth and wwidth are exactly the same (within their different units ofcourse). Also make sure that the image size is an odd number (so the central pixel is in the center). */ p->wwidth/=3600; /* Convert the width to degrees. */ twidth=p->wwidth/p->res; if(twidth<3) error(EXIT_FAILURE, 0, "--wwidth = %f (arcseconds) translates " "to %.0f pixels in scale of input image(s). This is probably " "not what you want", p->wwidth*3600, twidth); p->iwidth[0] = (twidth-(long)twidth)>0.5 ? twidth+1 : twidth; if(p->iwidth[0]%2==0) { p->iwidth[0]+=1; p->wwidth+=p->res; } p->iwidth[1]=p->iwidth[0]; } else if(p->res!=wcs->pc[3]) error(EXIT_FAILURE, 0, "%s: HDU %s: The resolution of " "this image is %f arcseconds/pixel while the " "previously checked input image(s) had a resolution " "of %f", img->name, p->cp.hdu, 3600*wcs->pc[3], 3600*p->res); /* Get the coordinates of the first pixel in the image. */ pixcrd[0]=1; pixcrd[1]=1; pixcrd[2]=img->naxes[0]; pixcrd[3]=1; pixcrd[4]=1; pixcrd[5]=img->naxes[1]; pixcrd[6]=img->naxes[0]; pixcrd[7]=img->naxes[1]; wcsp2s(wcs, ncoord, nelem, pixcrd, imgcrd, phi, theta, img->corners, &status); if(status) error(EXIT_FAILURE, 0, "wcsp2s ERROR %d: %s", status, wcs_errmsg[status]); /* Fill in the size of the image in celestial degrees from the first pixel in the image.*/ img->sized[0]=img->naxes[0]*p->res/cos(img->corners[1]*M_PI/180); img->sized[1]=img->naxes[1]*p->res; /* In case the image crosses the equator, we will calculate these values here so later on, we don't have to calculate them on every check. See the explanation above radecoverlap.*/ if( img->corners[1]*(img->corners[1]+img->sized[1]) < 0 ) { /* re in the explanations. */ img->equatorcorr[0]=img->corners[0] -0.5*img->sized[0]*(1-cos(img->corners[1]*M_PI/180)); /* sre in the explanations. */ img->equatorcorr[1]=img->sized[0]*cos(img->corners[1]*M_PI/180); } /* Just to check: printf("\n\n%s:\n(%.10f, %.10f)\n(%.10f, %.10f)" "\n(%.10f, %.10f)\n(%.10f, %.10f)\n\n", img->name, img->corners[0], img->corners[1], img->corners[2], img->corners[3], img->corners[4], img->corners[5], img->corners[6], img->corners[7]); exit(0); */ } /*******************************************************************/ /************ Check if WCS is in image **************/ /*******************************************************************/ /* Set the four sides around the point of interest in RA and Dec. NOTE: In this format we are working on here (where the image is aligned with the celestial coordinates), the declination is measured on a great circle, while the right ascension is not. So we have to consider the */ void setcsides(struct cropparams *crp) { size_t i; double h, hr, r, d, dr; /* The second r is for radians. */ struct imgcropparams *p=crp->p; double minra=FLT_MAX, mindec=FLT_MAX; double maxra=-FLT_MAX, maxdec=-FLT_MAX; /* Set the four corners of the WCS region. */ if(p->up.polygonset) { /* Find their minimum and maximum values. */ for(i=0;invertices;++i) { if(p->wpolygon[i*2]>maxra) maxra=p->wpolygon[i*2]; if(p->wpolygon[i*2]wpolygon[i*2]; if(p->wpolygon[i*2+1]>maxdec) maxdec=p->wpolygon[i*2+1]; if(p->wpolygon[i*2+1]wpolygon[i*2+1]; } /* Set the corners: */ crp->corners[0] = maxra; crp->corners[1] = mindec; /* Bottom Left */ crp->corners[2] = minra; crp->corners[3] = mindec; /* Bottom Right */ crp->corners[4] = maxra; crp->corners[5] = maxdec; /* Top Left */ crp->corners[6] = minra; crp->corners[7] = maxdec; /* Top Right */ } else { if(p->up.raset) { r=crp->world[0]=p->ra; d=crp->world[1]=p->dec; } else { r=crp->world[0]=p->cat[ crp->outindex * p->cs1 + p->racol ]; d=crp->world[1]=p->cat[ crp->outindex * p->cs1 + p->deccol ]; } h=p->wwidth/2; dr=d*M_PI/180; hr=h*M_PI/180; /* Set the four corners of this crop. */ crp->corners[0] = r+h/cos(dr-hr); crp->corners[1] = d-h; /* Bt Lf */ crp->corners[2] = r-h/cos(dr-hr); crp->corners[3] = d-h; /* Bt Rt */ crp->corners[4] = r+h/cos(dr+hr); crp->corners[5] = d+h; /* Tp Lf */ crp->corners[6] = r-h/cos(dr+hr); crp->corners[7] = d+h; /* Tp Rt */ } /* Set the bottom width and height of the crop in degrees. Note that the width changes as the height changes, so here we want the height and the lowest declination. Note that on the bottom edge, corners[0] is the maximum RA and corners[2] is the minimum RA. For all the region, corners[5] is one of the maximum declinations and corners[3] is one of the the minimum declinations.*/ crp->sized[0]=( (crp->corners[0]-crp->corners[2]) / cos(crp->corners[1]*M_PI/180) ); crp->sized[1]=crp->corners[5]-crp->corners[3]; /* In case the crop crosses the equator, then we need these two corrections. See the complete explanations below. */ if(crp->corners[1]*(crp->corners[1]+crp->sized[1]) < 0 ) { /* re in the explanations. */ crp->equatorcorr[0]=crp->corners[0] -0.5*crp->sized[0]*(1-cos(crp->corners[1]*M_PI/180)); /* sre in the explanations. */ crp->equatorcorr[1]=crp->sized[0]*cos(crp->corners[1]*M_PI/180); } /* Just to check: printf("\n\nCorner 1: (%.10f, %.10f)\n" "Corner 2: (%.10f, %.10f)\nCorner 3: (%.10f, %.10f)\n" "Corner 4: (%.10f, %.10f)\n\n", crp->corners[0], crp->corners[1], crp->corners[2], crp->corners[3], crp->corners[4], crp->corners[5], crp->corners[6], crp->corners[7]); */ } /* We have the polygon coordinates */ void fillcrpipolygon(struct cropparams *crp) { struct imgcropparams *p=crp->p; /* Allocate the array to keep the image based polygon sides */ errno=0; crp->ipolygon=malloc(2*p->nvertices*sizeof *crp->ipolygon); if(crp->ipolygon==NULL) error(EXIT_FAILURE, errno, "%zu bytes for crpp->ipolygon in " "onecrop (crop.c)", 2*p->nvertices*sizeof *crp->ipolygon); /* Fill in the crp->ipolygon array by converting the WCS polygon vertices to this image's coordinates. */ gal_wcs_radec_array_to_xy(p->imgs[crp->imgindex].wcs, p->wpolygon, crp->ipolygon, p->nvertices, 2); } /* BASICS: ======= An image is a rectangle, but the sky is on a globe. When the images are aligned to the celstial coordinates, (as we have required here in wcscheckprepare) the first FITS axis shows change in RA, while the second axis shows change in Dec. The declination always changes along a great circle, so there is no problem. But unless declination is constrained to zero, RA changes on small circles. See the rectangle below, assume it is an image. To check if a given point is within the same declination as this rectangle is very simple, since d3==d4 and d1==d2. Note that r1>r2 and r3>r4 (because right ascension increases to the east). (r3,d3) ------------------ (r4,d4) | | | | | | | | (r1,d1) ------------------ (r2,d2) But for RA, the same number of pixels on each declination, corresponds to different ranges in right ascention. As the declination gets higher in the northern hemisphere (where the declination rises towards the top of the image) r1-r2 becomes smaller than r3-r4. So, in terms of coverage in RA and Dec, this box should rather be shown like this trapezoid (exaggerated): -------------------- | | | | (Northern hemisphere) | | | | -------------- On the southern hemisphere it should be shown like this: ---------------- | | | | (Southern hemisphere) | | | | ---------------------- The functional form of the change is the inverse cosine, so: (r3-r4)=(r1-r2)/cos(d3-d1) (North) (r1-r2)=(r3-r4)/cos(d1-d3) (South) QUESTION: ======== Is a given point at the RA and Dec of (rp,dp) inside our rectangular image? IMAGE IS FULLY WITHIN ONE HEMISPHERE ------------------------------------ Our reference point for the image is the first pixel in the image, which by convention is the (r1,d1) point in the rectangle above. We also have the angular size of the rectangular image as 'sr', 'sd' (for "size in RA" and "size in dec"). NOTE: This has to be We also assume r1+sr and d1+sd are the distances to the last pixels in our rectangular image. As explained above, to check the declination range, everything is very easy: dp>=d1 && dp<=d1+sd For RA, things become a little more complicated (recall that r1>r3). `n` is defined as half of the extra space between the top and bottom lines of the two trapezoids. (North) n=0.5*sr*(1/cos(dp-d1)-1) ==> rp<=r1+n && rp>=r1-sr-n (South) n=0.5*sr*(1-cos(dp-d1)) ==> rp<=r1-n && rp>=r1-sr+n IMAGE CROSSES THE EQUATOR ------------------------- When d1*(d1+sd)<0, the image crosses the equator (d1 is negative and d1+sd is positive). In this case, we define `re` and `sre` as an equivalent of r1 and sr but on the equator: re=r1-0.5*sr*(1-cos(d1)) && sre=sr*cos(d1) then for all the points with negative declination we use the (South) equations of above as before and for those points that have a positive declination, we use the North formula but replacing r1 with re, d1 with 0 and sr with sre. */ /* p[2]: RA and Dec of a point (rp and dp above). i[2]: RA and Dec of first point in image. (r1 and d1 above). s[2]: Size of the image in degrees (sr and sd above). c[2]: Corrections if equator is passed, (se and sre above). */ int radecinimg(double *p, double *i, double *s, double *c) { double n; /* First check the declination. If it is not in range, you can safely return 0.*/ if(p[1]>=i[1] && p[1]<=i[1]+s[1]) { if(p[1]<=0) /* Point is in southern hemisphere, it */ { /* doesn't matter if image passes equator! */ n=0.5f*s[0]*( 1 - cos((p[1]-i[1])*M_PI/180) ); if(p[0]<=i[0]-n && p[0]>=i[0]-s[0]+n) return 1; } else /* Point is in the northern hemisphere. */ { if( i[1] * (s[1]+i[1]) > 0 ) /* Image does not cross equator. */ { n=0.5f*s[0]*( 1/cos((p[1]-i[1])*M_PI/180) - 1); if(p[0]<=i[0]+n && p[0]>=i[0]-s[0]-n) return 1; } else /* Image crosses the equator.*/ { n=0.5f*c[1]*( 1/cos((p[1] )*M_PI/180) - 1); if(p[0]<=c[0]+n && p[0]>=c[0]-c[1]-n) return 1; } } } return 0; } /* Is there an overlap between this crop box and the survey image? This function will return 0 if there isn't and 1 if there is. We don't want to necessarily assume that the crop box is smaller than the survey images. If we made that assumption, we only had to check if the corners of the crop are in the image. When we allow the input survey images to be smaller than the crop box, it might happen that none of the corners of the crop are in the image but there is an overlap (the survey image is completely within the crop box). So we have to check both. */ int radecoverlap(struct cropparams *crp) { double *d, *fd; double *i, *s, *c; /* for clear viewing. */ /* First check if the four sides of the crop box are in the image.*/ fd=(d=crp->corners)+8; s=crp->p->imgs[crp->imgindex].sized; i=crp->p->imgs[crp->imgindex].corners; c=crp->p->imgs[crp->imgindex].equatorcorr; do { if( radecinimg(d, i, s, c) ) return 1; d+=2; } while(dsized; i=crp->corners; c=crp->equatorcorr; fd=(d=crp->p->imgs[crp->imgindex].corners)+8; do { if( radecinimg(d, i, s, c) ) return 1; d+=2; } while(d Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef IMGMODE_H #define IMGMODE_H void imgcrop(struct imgcropparams *p); #endif gnuastro-0.2.33-8a3b/bin/imgcrop/imgcrop.c0000644000175000017500000002344613001632537015142 00000000000000/********************************************************************* ImageCrop - Crop a given size from one or multiple images. ImageCrop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include "main.h" #include "crop.h" #include "wcsmode.h" /* Write the log entry for each crop. A maximum length of FILENAME_BUFFER_IN_VERB characters is set for the filename to be displayed in stdout in verbose mode. This length is set to make the output on the user's terminal reasonable (in one line). So when the filename is longer than this, its first set of characters are truncated. In the log-file there is no truncation, therefore the log file should be used for checking the outputs, not the outputs printed on the screen. */ void reportcrop(struct imgcroplog *log) { size_t outnamelen=strlen(log->name);; char msg[GAL_TIMING_VERB_MSG_LENGTH_V]; /* Define the output string based on the length of the output file. */ if ( outnamelen > FILENAME_BUFFER_IN_VERB ) sprintf(msg, "...%s %zu %d", &log->name[ outnamelen - FILENAME_BUFFER_IN_VERB + 3 ], log->numimg, log->centerfilled); else sprintf(msg, "%-" MACROSTR(FILENAME_BUFFER_IN_VERB) "s %zu %d", log->name, log->numimg, log->centerfilled); gal_timing_report(NULL, msg, 2); } void * imgmodecrop(void *inparam) { struct cropparams *crp=(struct cropparams *)inparam; struct imgcropparams *p=crp->p; struct gal_commonparams *cp=&p->cp; size_t i; int status; struct inputimgs *img; struct imgcroplog *log; /* In image mode, we always only have one image. */ crp->imgindex=0; /* The whole catalog is from one image, so you can get the information here:*/ img=&p->imgs[crp->imgindex]; gal_fits_read_hdu(img->name, cp->hdu, 0, &crp->infits); /* Go over all the outputs that are assigned to this thread: */ for(i=0;crp->indexs[i]!=GAL_THREADS_NON_THRD_INDEX;++i) { /* Set all the output parameters: */ crp->outindex=crp->indexs[i]; log=&p->log[crp->outindex]; crp->outfits=NULL; log->numimg=0; cropname(crp); /* Crop the image. */ onecrop(crp); /* Check the final output: */ if(log->numimg) { /* Check if the center of the crop is filled or not. */ log->centerfilled=iscenterfilled(crp); /* Add the final headers and close output FITS image: */ gal_fits_write_keys_version(crp->outfits, NULL, SPACK_STRING); status=0; if( fits_close_file(crp->outfits, &status) ) gal_fits_io_error(status, "CFITSIO could not close " "the opened file"); /* Remove the output image if its center was not filled. */ if(log->centerfilled==0 && p->keepblankcenter==0) { errno=0; if(unlink(log->name)) error(EXIT_FAILURE, errno, "%s", log->name); } } else log->centerfilled=0; /* Report the status on stdout if verbose mode is requested. */ if(cp->verb) reportcrop(log); } /* Close the input image. */ status=0; if( fits_close_file(crp->infits, &status) ) gal_fits_io_error(status, "imgmode.c: imgcroponthreads could " "not close FITS file"); /* Wait until all other threads finish. */ if(cp->numthreads>1) pthread_barrier_wait(crp->b); return NULL; } void * wcsmodecrop(void *inparam) { struct cropparams *crp=(struct cropparams *)inparam; struct imgcropparams *p=crp->p; size_t i; int status, tcatset=0; struct imgcroplog *log; /* Go over all the output objects for this thread. */ for(i=0;crp->indexs[i]!=GAL_THREADS_NON_THRD_INDEX;++i) { /* Set all the output parameters: */ crp->outindex=crp->indexs[i]; log=&p->log[crp->outindex]; crp->outfits=NULL; log->name=NULL; log->numimg=0; /* Set the sides of the crop in RA and Dec */ setcsides(crp); /* Go over all the images to see if this target is within their range or not. */ crp->imgindex=0; do if(radecoverlap(crp)) { gal_fits_read_hdu(p->imgs[crp->imgindex].name, p->cp.hdu, 0, &crp->infits); if(log->name==NULL) cropname(crp); onecrop(crp); status=0; if( fits_close_file(crp->infits, &status) ) gal_fits_io_error(status, "imgmode.c: imgcroponthreads " "could not close FITS file"); } while ( ++(crp->imgindex) < p->numimg ); /* Check the final output: */ if(log->numimg) { log->centerfilled=iscenterfilled(crp); gal_fits_write_keys_version(crp->outfits, NULL, SPACK_STRING); status=0; if( fits_close_file(crp->outfits, &status) ) gal_fits_io_error(status, "CFITSIO could not close the " "opened file"); if(log->centerfilled==0 && p->keepblankcenter==0) { errno=0; if(unlink(log->name)) error(EXIT_FAILURE, errno, "%s", log->name); } } else { if(p->up.catset==0) /* Trick cropname into making a catalog */ { /* So we have a name for log report. */ tcatset=1; p->up.catset=1; } cropname(crp); if(tcatset) p->up.catset=0; log->centerfilled=0; } /* Report the status on stdout if verbose mode is requested. */ if(p->cp.verb) reportcrop(log); } /* Wait until all other threads finish. */ if(p->cp.numthreads>1) pthread_barrier_wait(crp->b); return NULL; } /*******************************************************************/ /************** Output function ****************/ /*******************************************************************/ /* Main function for the Image Mode. It is assumed that if only one crop box from each input image is desired, the first and last pixels are already set, irrespective of how the user specified that box. */ void imgcrop(struct imgcropparams *p) { int err=0; pthread_t t; /* We don't use the thread id, so all are saved here. */ pthread_attr_t attr; pthread_barrier_t b; struct cropparams *crp; size_t i, *indexs, thrdcols; size_t nt=p->cp.numthreads, nb; void *(*modefunction)(void *)=NULL; /* Set the function to run: */ if(p->imgmode) modefunction=&imgmodecrop; else if(p->wcsmode) modefunction=&wcsmodecrop; else error(EXIT_FAILURE, 0, "a bug! Somehow in imgcrop (imgcrop.c), " "neither the imgmode is on or the wcsmode! Please contact us " "so we can fix it, thanks"); /* Allocate the arrays to keep the thread and parameters for each thread. */ errno=0; crp=malloc(nt*sizeof *crp); if(crp==NULL) error(EXIT_FAILURE, errno, "%zu bytes in imgcrop (imgcrop.c) for crp", nt*sizeof *crp); /* Get the length of the output, no reasonable integer can have more than 50 characters! Since this is fixed for all the threads and images, we will just find it once here. */ crp[0].outlen=strlen(p->cp.output)+strlen(p->suffix)+50; /* Distribute the indexs into the threads (this is needed even if we only have one object where p->cs0 is not defined): */ if(p->up.catset) gal_threads_dist_in_threads(p->cs0, nt, &indexs, &thrdcols); else gal_threads_dist_in_threads(1, nt, &indexs, &thrdcols); /* Run the job, if there is only one thread, don't go through the trouble of spinning off a thread! */ if(nt==1) { crp[0].p=p; crp[0].indexs=indexs; modefunction(&crp[0]); } else { /* Initialize the attributes. Note that this running thread (that spinns off the nt threads) is also a thread, so the number the barrier should be one more than the number of threads spinned off. */ if(p->cs0cs0+1; else nb=nt+1; gal_threads_attr_barrier_init(&attr, &b, nb); /* Spin off the threads: */ for(i=0;icp.nolog==0) printlog(p); free(crp); free(indexs); } gnuastro-0.2.33-8a3b/bin/imgcrop/args.h0000644000175000017500000002527412774160624014455 00000000000000/********************************************************************* ImageCrop - Crop a given size from one or multiple images. ImageCrop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef ARGS_H #define ARGS_H #include #include #include /**************************************************************/ /************** argp.h definitions ***************/ /**************************************************************/ /* Definition parameters for the argp: */ const char *argp_program_version=SPACK_STRING"\n"GAL_STRINGS_COPYRIGHT "\n\nWritten by Mohammad Akhlaghi"; const char *argp_program_bug_address=PACKAGE_BUGREPORT; static char args_doc[] = "[ASCIIcatalog] ASTRdata ..."; const char doc[] = /* Before the list of options: */ GAL_STRINGS_TOP_HELP_INFO SPACK_NAME" will create cutouts, thumbnails, postage stamps or crops of " "region(s) from input image(s) using image or celestial coordinates. " "If muliple crops are desired, a catalog must be provided. When in WCS " "mode, if the cut out covers more than one input image, all overlapping " "input images will be stitched in the output.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /* Available letters for short options: e m n t u v A B C E F G H J L M O Q R T U X Y Z Number keys used<=502 Options with keys (second structure element) larger than 500 do not have a short version. */ static struct argp_option options[] = { { 0, 0, 0, 0, "Operating modes:", -1 }, { "imgmode", 'I', 0, 0, "Use image coordinates (x and y).", -1 }, { "wcsmode", 'W', 0, 0, "Use WCS coordinates (Ra and Dec).", -1 }, { 0, 0, 0, 0, "Input:", 1 }, { "hstartwcs", 501, "INT", 0, "Header keyword number to start reading WCS.", 1 }, { "hendwcs", 502, "INT", 0, "Header keyword number to stop reading WCS.", 1 }, { 0, 0, 0, 0, "Output:", 2 }, { "noblank", 'b', 0, 0, "Remove parts of the crop box out of input image.", 2 }, { "keepblankcenter", 'k', 0, 0, "Keep crop if the central parts are not filled.", 2 }, { "checkcenter", 'c', "INT", 0, "Side of box (in pixels) to check.", 2 }, { "suffix", 'p', "STR", 0, "Suffix (postfix) of cropped images.", 2 }, { 0, 0, 0, 0, "Crop:", 3 }, { "racol", 'f', "INT", 0, "Column of Right Ascension (RA) in catalog.", 3 }, { "deccol", 'g', "INT", 0, "Column of Declination (Dec) in catalog.", 3 }, { "ra", 'r', "FLT", 0, "Right ascension of one crop box center.", 3 }, { "dec", 'd', "FLT", 0, "Declination of one crop box center.", 3 }, { "xcol", 'i', "INT", 0, "Column of X (first FITS axis) value in catalog.", 3 }, { "ycol", 'j', "INT", 0, "Column of Y (second FITS axis) in catalog.", 3 }, { "xc", 'x', "FLT", 0, "First axis position for only one crop.", 3 }, { "yc", 'y', "FLT", 0, "Second axis position for only one crop.", 3, }, { "iwidth", 'a', "INT", 0, "Image mode width (in pixels).", 3 }, { "wwidth", 'w', "FLT", 0, "WCS mode width (in arc seconds).", 3 }, { "section", 's', "STR", 0, "Image section string specifying crop range.", 3 }, { "polygon", 'l', "STR", 0, "Polygon vertices of region to crop.", 3 }, { "outpolygon", 500, 0, 0, "Keep the polygon's outside, mask the inside.", 3 }, { "zeroisnotblank", 'z', 0, 0, "0.0 in float or double images are not blank.", 3 }, {0} }; /* Parse a single option: */ static error_t parse_opt(int key, char *arg, struct argp_state *state) { /* A temporary variable. */ size_t tmp; /* Save the arguments structure: */ struct imgcropparams *p = state->input; /* Set the pointer to the common parameters for all programs here: */ state->child_inputs[0]=&p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); switch(key) { /* Operating modes: */ case 'I': if(p->up.imgmodeset) argp_error(state, "only one of Image or WCS modes can be chosen"); p->imgmode=1; p->wcsmode=0; p->up.imgmodeset=p->up.wcsmodeset=1; break; case 'W': if(p->up.wcsmodeset) argp_error(state, "only one of Image or WCS modes can be chosen"); p->imgmode=0; p->wcsmode=1; p->up.imgmodeset=p->up.wcsmodeset=1; break; /* Input */ case 501: gal_checkset_sizet_el_zero(arg, &p->hstartwcs, "hstartwcs", key, SPACK, NULL, 0); p->up.hstartwcsset=1; break; case 502: gal_checkset_sizet_el_zero(arg, &p->hendwcs, "hendwcs", key, SPACK, NULL, 0); p->up.hendwcsset=1; break; /* Output parameters: */ case 'b': p->noblank=1; break; case 'k': p->keepblankcenter=1; break; case 'c': gal_checkset_sizet_l_zero(arg, &p->checkcenter, "checkcenter", key, SPACK, NULL, 0); p->up.checkcenterset=1; break; case 'p': gal_checkset_allocate_copy_set(arg, &p->suffix, &p->up.suffixset); break; /* Crop: */ case 'f': gal_checkset_sizet_el_zero(arg, &p->racol, "racol", key, SPACK, NULL, 0); p->up.racolset=1; break; case 'g': gal_checkset_sizet_el_zero(arg, &p->deccol, "deccol", key, SPACK, NULL, 0); p->up.deccolset=1; break; case 'r': gal_checkset_any_double(arg, &p->ra, "ra", key, SPACK, NULL, 0); p->up.raset=1; break; case 'd': gal_checkset_any_double(arg, &p->dec, "dec", key, SPACK, NULL, 0); p->up.decset=1; break; case 'i': gal_checkset_sizet_el_zero(arg, &p->xcol, "xcol", key, SPACK, NULL, 0); p->up.xcolset=1; break; case 'j': gal_checkset_sizet_el_zero(arg, &p->ycol, "ycol", key, SPACK, NULL, 0); p->up.ycolset=1; break; case 'x': gal_checkset_any_double(arg, &p->xc, "xc", key, SPACK, NULL, 0); p->up.xcset=1; /* Using FITS standard, not C. */ break; case 'y': gal_checkset_any_double(arg, &p->yc, "yc", key, SPACK, NULL, 0); p->up.ycset=1; /* Using FITS standard, not C. */ break; case 'a': gal_checkset_sizet_l_zero(arg, &tmp, "iwidth", key, SPACK, NULL, 0); p->iwidth[0]=p->iwidth[1]=tmp; p->up.iwidthset=1; break; case 'w': gal_checkset_double_l_0(arg, &p->wwidth, "wwidth", key, SPACK, NULL, 0); p->up.wwidthset=1; break; case 's': p->section=arg; p->up.sectionset=1; break; case 'l': p->up.polygon=arg; p->up.polygonset=1; break; case 500: p->outpolygon=1; break; case 'z': p->zeroisnotblank=1; break; /* Read the non-option arguments: */ case ARGP_KEY_ARG: /* See what type of input value it is and put it in. */ if( gal_fits_name_is_fits(arg) ) { gal_linkedlist_add_to_stll(&p->up.gal_linkedlist_stll, arg); ++p->numimg; } else { if(p->up.catname) argp_error(state, "only one catalog file can be given"); else { p->up.catname=arg; p->up.catset=1; } } break; /* The command line options and arguments are finished. */ case ARGP_KEY_END: if(p->cp.setdirconf==0 && p->cp.setusrconf==0 && p->cp.printparams==0) { if(state->arg_num==0) argp_error(state, "no argument given"); if(p->up.catname==NULL && !(p->up.xcset || p->up.ycset || p->up.raset || p->up.decset || p->up.sectionset || p->up.polygonset)) argp_error(state, "no catalog provided"); if(p->up.gal_linkedlist_stll==NULL) argp_error(state, "no FITS image(s) provided"); } break; default: return ARGP_ERR_UNKNOWN; } return 0; } /* Specify the children parsers: */ struct argp_child children[]= { {&commonargp, 0, NULL, 0}, {0, 0, 0, 0} }; /* Basic structure defining the whole argument reading process. */ static struct argp thisargp = {options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif gnuastro-0.2.33-8a3b/bin/imgcrop/ui.h0000644000175000017500000000223412616616510014120 00000000000000/********************************************************************* ImageCrop - Crop a given size from one or multiple images. ImageCrop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef IMCROPUI_H #define IMCROPUI_H void setparams(int argc, char *argv[], struct imgcropparams *p); void freeandreport(struct imgcropparams *p, struct timeval *t1); #endif gnuastro-0.2.33-8a3b/bin/imgcrop/ui.c0000644000175000017500000005656613001632537014130 00000000000000/********************************************************************* ImageCrop - Crop a given size from one or multiple images. ImageCrop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include /* From Gnulib. */ #include /* Includes time.h and sys/time.h */ #include #include #include #include "main.h" #include "crop.h" #include "wcsmode.h" #include "ui.h" /* Needs main.h */ #include "args.h" /* Needs main.h, includes argp.h. */ /* Set the file names of the places where the default parameters are put. */ #define CONFIG_FILE SPACK CONF_POSTFIX #define SYSCONFIG_FILE SYSCONFIG_DIR "/" CONFIG_FILE #define USERCONFIG_FILEEND USERCONFIG_DIR CONFIG_FILE #define CURDIRCONFIG_FILE CURDIRCONFIG_DIR CONFIG_FILE /**************************************************************/ /************** Options and parameters ***************/ /**************************************************************/ void readconfig(char *filename, struct imgcropparams *p) { FILE *fp; int zeroorone; char *line, *name, *value; struct uiparams *up=&p->up; size_t lineno=0, len=200, tmp; struct gal_commonparams *cp=&p->cp; char key='a'; /* Not used, just a place holder. */ int imgmodeset=0, wcsmodeset=0; /* Unambiguous default file checking. */ /* When the file doesn't exist or can't be opened, it is ignored. It might be intentional, so there is no error. If a parameter is missing, it will be reported after all defaults are read. */ fp=fopen(filename, "r"); if (fp==NULL) return; /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); /* Read the tokens in the file: */ while(getline(&line, &len, fp) != -1) { /* Prepare the "name" and "value" strings, also set lineno. */ GAL_CONFIGFILES_START_READING_LINE; /* Operating modes: */ if(strcmp(name, "imgmode")==0) { gal_checkset_int_zero_or_one(value, &zeroorone, name, key, SPACK, filename, lineno); if(zeroorone) { imgmodeset=1; if(wcsmodeset) error_at_line(EXIT_FAILURE, 0, filename, lineno, "Image and WCS modes cannot be called " "together. It is ambiguous."); if(up->imgmodeset==0) { p->imgmode=1; p->wcsmode=0; up->imgmodeset=up->wcsmodeset=1; } } } else if(strcmp(name, "wcsmode")==0) { gal_checkset_int_zero_or_one(value, &zeroorone, name, key, SPACK, filename, lineno); if(zeroorone) { wcsmodeset=1; if(imgmodeset) error_at_line(EXIT_FAILURE, 0, filename, lineno, "Image and WCS modes cannot be called " "together. It is ambiguous."); if(up->wcsmodeset==0) { p->imgmode=0; p->wcsmode=1; up->imgmodeset=up->wcsmodeset=1; } } } /* Inputs: */ else if(strcmp(name, "hdu")==0) gal_checkset_allocate_copy_set(value, &cp->hdu, &cp->hduset); else if(strcmp(name, "racol")==0) { if(up->racolset) continue; gal_checkset_sizet_el_zero(value, &p->racol, name, key, SPACK, filename, lineno); up->racolset=1; } else if(strcmp(name, "deccol")==0) { if(up->deccolset) continue; gal_checkset_sizet_el_zero(value, &p->deccol, name, key, SPACK, filename, lineno); up->deccolset=1; } else if(strcmp(name, "xcol")==0) { if(up->xcolset) continue; gal_checkset_sizet_el_zero(value, &p->xcol, name, key, SPACK, filename, lineno); up->xcolset=1; } else if(strcmp(name, "ycol")==0) { if(up->ycolset) continue; gal_checkset_sizet_el_zero(value, &p->ycol, name, key, SPACK, filename, lineno); up->ycolset=1; } else if(strcmp(name, "iwidth")==0) { if(up->iwidthset) continue; gal_checkset_sizet_l_zero(value, &tmp, name, key, SPACK, filename, lineno); p->iwidth[0]=p->iwidth[1]=tmp; up->iwidthset=1; } else if(strcmp(name, "wwidth")==0) { if(up->wwidthset) continue; gal_checkset_double_l_0(value, &p->wwidth, name, key, SPACK, filename, lineno); up->wwidthset=1; } else if(strcmp(name, "hstartwcs")==0) { if(up->hstartwcsset) continue; gal_checkset_sizet_el_zero(value, &p->hstartwcs, name, key, SPACK, filename, lineno); up->hstartwcsset=1; } else if(strcmp(name, "hendwcs")==0) { if(up->hendwcsset) continue; gal_checkset_sizet_el_zero(value, &p->hendwcs, name, key, SPACK, filename, lineno); up->hendwcsset=1; } /* Outputs */ else if(strcmp(name, "checkcenter")==0) { if(up->checkcenterset) continue; gal_checkset_sizet_el_zero(value, &p->checkcenter, name, key, SPACK, filename, lineno); up->checkcenterset=1; } else if(strcmp(name, "output")==0) gal_checkset_allocate_copy_set(value, &cp->output, &cp->outputset); else if(strcmp(name, "suffix")==0) gal_checkset_allocate_copy_set(value, &p->suffix, &up->suffixset); /* Read options common to all programs */ GAL_CONFIGFILES_READ_COMMONOPTIONS_FROM_CONF else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s` not recognized.\n", name); } free(line); fclose(fp); } void printvalues(FILE *fp, struct imgcropparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; /* Print all the options that are set. Separate each group with a commented line explaining the options in that group. */ fprintf(fp, "\n# Input image:\n"); if(cp->hduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("hdu", cp->hdu); fprintf(fp, "\n# Output parameters:\n"); if(up->checkcenterset) fprintf(fp, CONF_SHOWFMT"%zu\n", "checkcenter", p->checkcenter); if(cp->outputset) fprintf(fp, CONF_SHOWFMT"%s\n", "output", cp->output); if(up->suffixset) fprintf(fp, CONF_SHOWFMT"%s\n", "suffix", p->suffix); fprintf(fp, "\n# Crop parameters:\n"); if(up->xcolset) fprintf(fp, CONF_SHOWFMT"%zu\n", "xcol", p->xcol); if(up->ycolset) fprintf(fp, CONF_SHOWFMT"%zu\n", "ycol", p->ycol); if(up->iwidthset) fprintf(fp, CONF_SHOWFMT"%ld\n", "iwidth", p->iwidth[0]); if(up->racolset) fprintf(fp, CONF_SHOWFMT"%zu\n", "racol", p->racol); if(up->deccolset) fprintf(fp, CONF_SHOWFMT"%zu\n", "deccol", p->deccol); if(up->wwidthset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "wwidth", p->wwidth); if(up->hstartwcsset) fprintf(fp, CONF_SHOWFMT"%zu\n", "hstartwcs", p->hstartwcs); if(up->hendwcsset) fprintf(fp, CONF_SHOWFMT"%zu\n", "hendwcs", p->hendwcs); /* For the operating mode, first put the macro to print the common options, then the (possible options particular to this program). */ fprintf(fp, "\n# Operating mode:\n"); GAL_CONFIGFILES_PRINT_COMMONOPTIONS; if(up->imgmodeset) fprintf(fp, CONF_SHOWFMT"%d\n", "imgmode", p->imgmode); if(up->wcsmodeset) fprintf(fp, CONF_SHOWFMT"%d\n", "wcsmode", p->wcsmode); } /* Note that numthreads will be used automatically based on the configure time. */ void checkifset(struct imgcropparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; int intro=0; if(up->imgmodeset==0 && up->wcsmodeset==0) GAL_CONFIGFILES_REPORT_NOTSET("imgmode or wcsmode"); if(cp->hduset==0) GAL_CONFIGFILES_REPORT_NOTSET("hdu"); if(up->xcolset==0) GAL_CONFIGFILES_REPORT_NOTSET("xcol"); if(up->ycolset==0) GAL_CONFIGFILES_REPORT_NOTSET("ycol"); if(up->iwidthset==0) GAL_CONFIGFILES_REPORT_NOTSET("iwidth"); if(up->racolset==0) GAL_CONFIGFILES_REPORT_NOTSET("racol"); if(up->deccolset==0) GAL_CONFIGFILES_REPORT_NOTSET("deccol"); if(up->wwidthset==0) GAL_CONFIGFILES_REPORT_NOTSET("wwidth"); if(up->suffixset==0) GAL_CONFIGFILES_REPORT_NOTSET("suffix"); if(up->checkcenterset==0) GAL_CONFIGFILES_REPORT_NOTSET("checkcenter"); GAL_CONFIGFILES_END_OF_NOTSET_REPORT; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ void sanitycheck(struct imgcropparams *p) { int checksum; char forerr[100]; struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; /* checkcenter is odd: */ if(p->checkcenter%2==0) p->checkcenter+=1; /* Width and checkcenter are odd */ if(p->iwidth[0]<3) error(EXIT_FAILURE, 0, "--iwidth has to be 3 or more pixels"); else if(p->iwidth[0]%2==0) p->iwidth[0]+=1; p->iwidth[1]=p->iwidth[0]; if(p->checkcenter<3) error(EXIT_FAILURE, 0, "--checkcenter has to be 3 or more pixels"); else if(p->checkcenter%2==0) p->checkcenter+=1; /* deccol!=racol and xcol!=ycol */ if(p->racol==p->deccol) error(EXIT_FAILURE, 0, "the columns for RA and Dec must be " "different"); if(p->xcol==p->ycol) error(EXIT_FAILURE, 0, "the columns for x and y must be " "different"); /* Make sure that if any of --ra or --dec are given, the other is also given. */ checksum=up->raset+up->decset; if(checksum==2) {p->imgmode=0; p->wcsmode=1;} else if(checksum)/* is not zero */ error(EXIT_FAILURE, 0, "the options `--ra` and `--dec` should be " "called together"); /* Make sure that if any of --xc or --yc are given, the other is also given. */ checksum=up->xcset+up->ycset; if(checksum==2) {p->imgmode=1; p->wcsmode=0;} else if(checksum)/* is not zero */ error(EXIT_FAILURE, 0, "the options `--xc` and `--yc` should be " "called together"); /* --section is given, it goes into image mode: */ if(up->sectionset) {p->imgmode=1; p->wcsmode=0;} /* Make sure that the multiple one crop box options have not been called together. */ checksum=up->raset+up->xcset+up->sectionset+up->polygonset; if(checksum) { /* Only one of the three should be called. */ if(checksum!=1) { forerr[0]='\0'; if(up->raset) strcat(forerr, "(`--ra' and `--dec'), "); if(up->xcset) strcat(forerr, "(`--xc' and `--yc'), "); if(up->sectionset) strcat(forerr, "(`--section'), "); if(up->polygonset) strcat(forerr, "(`--polygon'), "); error(EXIT_FAILURE, 0, "there are several ways to specify a crop " "box on the command line, see `--help`. But they should " "not be called together. You have asked for %s " "simultaneously", forerr); } /* Check if the value for --output is a file or a directory? */ p->outnameisfile=gal_checkset_dir_0_file_1(cp->output, cp->dontdelete); /* When there is only one output, only one thread is needed. */ cp->numthreads=1; /* Not with a catalog. */ if(up->catname) { if(up->sectionset) strcpy(forerr, "`--section'"); if(up->polygonset) strcpy(forerr, "`--polygon'"); if(up->xcset) strcpy(forerr, "`--xc' and `--yc'"); if(up->raset) strcpy(forerr, "`--ra' and `--dec'"); error(EXIT_FAILURE, 0, "a catalog name (%s) and command line " "crop parameters (%s) cannot be given together", up->catname, forerr); } } else { /* Only one mode. Note that when the box is specified on the command line, in the steps above, we set the image mode or wcs mode.*/ if(p->imgmode && p->wcsmode) error(EXIT_FAILURE, 0, "only one of imgmode or wcsmode " "must be called. They cannot operate together"); else if(p->imgmode==0 && p->wcsmode==0) error(EXIT_FAILURE, 0, "at least one of imgmode or " "wcsmode must be called"); /* Make sure a catalog is set. */ if(up->catset) { if(p->numimg>1 && p->imgmode) error(EXIT_FAILURE, 0, "in image mode, when a catalog is " "specified, only one image may be provided"); } else error(EXIT_FAILURE, 0, "no catalog. When no crop coordinates " "are specified on the command line, a catalog must be " "provided"); /* Make sure the given output is a directory. */ gal_checkset_check_dir_write_add_slash(&cp->output); /* Make sure the columns of data are within the catalog range of columns: */ if(p->imgmode) { GAL_CHECKSET_CHECK_COL_IN_CAT(p->xcol, "xcol"); GAL_CHECKSET_CHECK_COL_IN_CAT(p->ycol, "ycol"); } else { GAL_CHECKSET_CHECK_COL_IN_CAT(p->racol, "racol"); GAL_CHECKSET_CHECK_COL_IN_CAT(p->deccol, "deccol"); } } /* If in image mode, there should only be one input image. */ if(p->imgmode && p->numimg>1) error(EXIT_FAILURE, 0, "in image mode, only one input image may be " "specified"); /* If we are in WCS mode, noblanks must be off */ if(p->wcsmode && p->noblank) error(EXIT_FAILURE, 0, "`--noblanks` (`-b`) is only for image mode. " "You have called it with WCS mode"); /* Parse the polygon vertices if they are given to make sure that there is no error: */ if(p->up.polygonset) { polygonparser(p); if(p->nvertices<3) error(EXIT_FAILURE, 0, "a polygon has to have 3 or more vertices, " "you have only given %zu (%s)", p->nvertices, p->up.polygon); if(p->outpolygon && p->numimg>1) error(EXIT_FAILURE, 0, "currently in WCS mode, outpolygon can only " "be set to zero when there is one image, you have given %zu " "images. For multiple images the region will be very large. " "It is best if you first crop out the larger region you want " "into one image, then mask the polygon", p->numimg); } else p->wpolygon=p->ipolygon=NULL; /* Check that if multiple threads are beeing requested, CFITSIO is configured with the `--enable-reentrant` option. This is put here because the number of threads may change above. */ if(cp->numthreads>1 && fits_is_reentrant()==0) error(EXIT_FAILURE, 0, "CFITSIO was not configured with the " "`--enable-reentrant` option but you have asked to operate " "on %zu threads. Please configure, make and install CFITSIO " "again with this flag to use multiple threads, run `info %s " "CFITSIO` for more information. Alternatively you can set " "the number of threads to 1 by adding the `--numthreads=1` " "or `-N1` options", cp->numthreads, PACKAGE); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ /* It is important that the image names are stored in an array (for WCS mode in particular). We do that here. */ void preparearrays(struct imgcropparams *p) { size_t size, num; fitsfile *tmpfits; struct timeval t1; struct inputimgs *img; int i, status, firstbitpix=0; char msg[GAL_TIMING_VERB_MSG_LENGTH_V]; if(p->cp.verb) gettimeofday(&t1, NULL); /* Fill in the WCS information of each image. This is done here because WCSLIB is unfortunately not thread-safe when reading the WCS information from the FITS files. In cases where the number of cropped images are more than the input images, this can also be a preformance boost because each image information is only read once. The images are filled in opposite order because we used a linked list to read them in, which is a first in first out structure.*/ errno=0; size=p->numimg*sizeof *p->imgs; p->imgs=malloc(size); if(p->imgs==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes for p->imgs", size); for(i=p->numimg-1;i>=0;--i) { /* Get the image properties. */ status=0; img=&p->imgs[i]; gal_linkedlist_pop_from_stll(&p->up.gal_linkedlist_stll, &img->name); gal_fits_read_hdu(img->name, p->cp.hdu, 0, &tmpfits); gal_fits_img_bitpix_size(tmpfits, &p->bitpix, img->naxes); gal_fits_read_wcs_from_pointer(tmpfits, &img->nwcs, &img->wcs, p->hstartwcs, p->hendwcs); if(img->wcs) { status=wcshdo(0, img->wcs, &img->nwcskeys, &img->wcstxt); if(status) error(EXIT_FAILURE, 0, "wcshdo ERROR %d: %s", status, wcs_errmsg[status]); } else if(p->wcsmode) error(EXIT_FAILURE, 0, "the WCS structure of %s (hdu: %s) " "image is not recognized. So RA and Dec cannot be used " "as input. You can try with pixel coordinates in the " "Image Mode (note that the crops will lack WCS " "header information)", img->name, p->cp.hdu); fits_close_file(tmpfits, &status); gal_fits_io_error(status, NULL); /* Make sure all the images have the same BITPIX and set the basic BITPIX related parameters. */ if(firstbitpix==0) { firstbitpix=p->bitpix; p->datatype=gal_fits_bitpix_to_datatype(p->bitpix); p->bitnul=gal_fits_datatype_blank(p->datatype); } else if(firstbitpix!=p->bitpix) error(EXIT_FAILURE, 0, "%s: BITPIX=%d. Previous images had a " "BITPIX value of %d, For "SPACK_NAME" to work, all images " "must have the same pixel data type", img->name, p->bitpix, firstbitpix); /* In WCS mode, Check resolution and get the first pixel positions. */ if(p->wcsmode) wcscheckprepare(p, img); } /* Array of log structures. We will make one more than the needed numbers so that we can put a NULL character in the name section of it to sign its end (something like a string). This is done so we don't have to worry about the length calculation any more! */ if(p->up.xcset || p->up.sectionset || p->up.raset || p->up.polygonset) num=1; else num=p->cs0; errno=0; p->log=calloc(num+1, sizeof *p->log); if(p->log==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes for p->log", num+1 * sizeof *p->log); /* Report timing: */ if(p->cp.verb) { sprintf(msg, "Read metadata of %zu images.", p->numimg); gal_timing_report(&t1, msg, 1); } } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void setparams(int argc, char *argv[], struct imgcropparams *p) { struct gal_commonparams *cp=&p->cp; /* Set the non-zero initial values, the structure was initialized to have a zero value for all elements. */ cp->spack = SPACK; cp->verb = 1; cp->numthreads = num_processors(NPROC_CURRENT); cp->removedirinfo = 1; /* Read the arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Add the user default values and save them if asked. */ GAL_CONFIGFILES_CHECK_SET_CONFIG; /* Check if all the required parameters are set. */ checkifset(p); /* Print the values for each parameter. */ if(cp->printparams) GAL_CONFIGFILES_REPORT_PARAMETERS_SET; /* Read catalog if given. */ if(p->up.catname) gal_txtarray_txt_to_array(p->up.catname, &p->cat, &p->cs0, &p->cs1); /* If cp->output was not specified on the command line or in any of the configuration files, then automatic output should be used, in which case, cp->output should be the current directory. */ if(p->cp.outputset==0) { p->cp.output=malloc(2+1); /* 2 is length of "./" */ if(p->cp.output==NULL) error(EXIT_FAILURE, errno, "space for output"); strcpy(p->cp.output, "./"); p->cp.outputset=1; } /* Do a sanity check. */ sanitycheck(p); gal_checkset_check_remove_file(GAL_TXTARRAY_LOG, 0); /* Everything is ready, notify the user of the program starting. */ if(cp->verb) printf(SPACK_NAME" started on %s", ctime(&p->rawtime)); /* Make the array of input images. */ preparearrays(p); } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void freeandreport(struct imgcropparams *p, struct timeval *t1) { size_t i; int status; /* Free the allocated arrays: */ free(p->cat); free(p->cp.hdu); free(p->bitnul); free(p->suffix); free(p->wpolygon); free(p->ipolygon); /* If these two pointers point to the same place,, that plce will be freed below. */ if(p->log[0].name != p->cp.output) free(p->cp.output); /* Free the allocated WCS parameters: */ for(i=0;inumimg;++i) if(p->imgs[i].wcs) { free(p->imgs[i].wcstxt); status=wcsvfree(&p->imgs[i].nwcs, &p->imgs[i].wcs); if(status) error(EXIT_FAILURE, 0, "wcsvfree ERROR %d: %s", status, wcs_errmsg[status]); } free(p->imgs); /* Free the log array: */ for(i=0;p->log[i].name;++i) free(p->log[i].name); free(p->log); /* Print the final message. */ if(p->cp.verb) gal_timing_report(t1, SPACK_NAME" finished in: ", 0); } gnuastro-0.2.33-8a3b/bin/imgcrop/cite.h0000644000175000017500000000317512750745735014447 00000000000000/********************************************************************* ImageCrop - Crop a given size from one or multiple images. ImageCrop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CITE_H #define CITE_H #define IMGCROPBIBTEX "" #define PRINTCITEABORT { \ printf("\nWe hope %s has been useful for your research.\n" \ "Citations are vital for the continued work on %s.\n" \ "Thank you for citing it in your research paper.\n" \ "\nPlease cite as \"%s\":\n\n%s\n\n%s", \ SPACK_NAME, SPACK_NAME, SPACK_STRING, \ GAL_STRINGS_MAIN_BIBTEX, IMGCROPBIBTEX); \ exit(EXIT_SUCCESS); \ } #endif gnuastro-0.2.33-8a3b/bin/imgcrop/main.h0000644000175000017500000001606212774156733014446 00000000000000/********************************************************************* ImageCrop - Crop a given size from one or multiple images. ImageCrop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include #include #include /* Progarm name macros: */ #define SPACK "astimgcrop" /* Subpackage executable name. */ #define SPACK_NAME "ImageCrop" /* Subpackage full name. */ #define SPACK_STRING SPACK_NAME" ("PACKAGE_NAME") "PACKAGE_VERSION #define LOGFILENAME SPACK".log" /* Set the maximum length given to a file name when run in verbose mode. The STR macro function is used to convert the numerical macro value into a string (which is necessary). STR_HELPER(x) uses the C pre-processor's "stringification" functionality. See the "Stringification" section of the GNU C Pre-Processor manual for a thorough explanation. Note that this is part of the C standard, not just GNU C. */ #define STRINGIFY(x) #x #define MACROSTR(x) STRINGIFY(x) #define FILENAME_BUFFER_IN_VERB 30 /* Structure for the log file. Since we are operating in parallel mode, writing to a file will significantly decrease the speed. So we will make an array to keep the status of each output.*/ struct imgcroplog { char *name; /* The name of this output. */ size_t numimg; /* The number of images used in this output. */ int centerfilled; /* Is the center filled? (0 or 1) */ }; /* The sides of the image keep the celestial coordinates of the four sides of this image. With respect to the pixels they are. */ struct inputimgs { char *name; /* File name of input image. */ long naxes[2]; /* Size of the image. */ int nwcs; /* Number of WCS in each input image. */ struct wcsprm *wcs; /* WCS structure of each input image. */ char *wcstxt; /* Text output of each WCS. */ int nwcskeys; /* Number of keywords in the header WCS. */ double corners[8]; /* RA and Dec of this image corners (within). */ double sized[2]; /* Width and height of image in degrees. */ double equatorcorr[2]; /* If image crosses the equator, see wcsmode.c.*/ }; /* User interface parameters: */ struct uiparams { char *catname; /* Catalog file name. */ struct gal_linkedlist_stll *gal_linkedlist_stll; /* Input file names. */ char *polygon; /* String of input polygon vertices. */ /* Check if all parameters are read (use .def file for comparison). The non optional parameters (like the catalog and input FITS images that come in from arguments, not options) are checked in the args.h files. */ int catset; int imgmodeset; int wcsmodeset; int racolset; int deccolset; int raset; int decset; int xcolset; int ycolset; int xcset; int ycset; int iwidthset; int wwidthset; int sectionset; int polygonset; int suffixset; int checkcenterset; int hstartwcsset; int hendwcsset; }; /* Main program parameters: */ struct imgcropparams { /* Before actual program: */ struct uiparams up; /* User interface parameters. */ struct gal_commonparams cp; /* Common parameters. */ /* Operating modes: */ int imgmode; /* ==1: will use X and Y coordiates. */ int wcsmode; /* ==1: will use Ra and Dec coordiates. */ /* Input */ size_t numimg; /* Number of given image names. */ size_t xcol; /* Catalog X column */ size_t ycol; /* Catalog Y column */ int noblank; /* ==1: no blank (out of image) pixels. */ char *section; /* Section string. */ double *wpolygon; /* Array of WCS polygon vertices. */ double *ipolygon; /* Array of image polygon vertices. */ size_t nvertices; /* Number of polygon vertices. */ double xc; /* The center point, one crop (FITS stnrd). */ double yc; /* The center point, one crop (FITS stnrd). */ long iwidth[2]; /* Image mode width (in pixels). */ size_t racol; /* Catalog RA column */ size_t deccol; /* Catalog Dec column */ double ra; /* RA of one crop box center. */ double dec; /* Dec of one crop box center. */ double res; /* Resolution in arcseconds */ double wwidth; /* WCS mode width (in arcseconds). */ size_t checkcenter; /* width of a box to check for zeros */ int keepblankcenter; /* ==1: If center is not filled, remove. */ int zeroisnotblank; /* ==1: In float or double, keep 0.0 pixels.*/ int outpolygon; /* ==1: Keep the inner polygon region. */ size_t hstartwcs; /* Header keyword No. to start reading WCS. */ size_t hendwcs; /* Header keyword No. to end reading WCS. */ /* Output: */ char *suffix; /* Ending of output file name. */ /* INTERNAL PARAMETERS: */ struct inputimgs *imgs; /* Basic WCS and size information for input.*/ struct imgcroplog *log; /* To keep the log of the outputs. */ time_t rawtime; /* Starting time of the program. */ int outnameisfile; /* Output filename is a directory. */ double *cat; /* Data of catalog. */ size_t cs0; /* Number of rows in the catalog. */ size_t cs1; /* Number of columns in the catalog. */ int bitpix; /* BITPIX value for all images. */ void *bitnul; /* Null value for this data-type. */ int datatype; /* CFITSIO datatype value for this image. */ }; /* Function declarations: */ void imgcrop(struct imgcropparams *p); #endif gnuastro-0.2.33-8a3b/bin/imgcrop/main.c0000644000175000017500000000314212774156733014434 00000000000000/********************************************************************* ImageCrop - Crop a given size from one or multiple images. ImageCrop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include /* Includes time.h and sys/time.h */ #include "main.h" #include "imgcrop.h" #include "ui.h" /* needs main.h. */ int main (int argc, char *argv[]) { struct timeval t1; struct imgcropparams p={{0}, {0}, 0}; /* Set the starting time.*/ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ setparams(argc, argv, &p); /* Run Image Crop */ imgcrop(&p); /* Free all non-freed allocations. */ freeandreport(&p, &t1); /* Return successfully.*/ return EXIT_SUCCESS; } gnuastro-0.2.33-8a3b/bin/imgcrop/Makefile.in0000644000175000017500000017303713004464626015412 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without 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GNULIB_BTOWC = @GNULIB_BTOWC@ GNULIB_CALLOC_POSIX = @GNULIB_CALLOC_POSIX@ GNULIB_CANONICALIZE_FILE_NAME = @GNULIB_CANONICALIZE_FILE_NAME@ GNULIB_CBRT = @GNULIB_CBRT@ GNULIB_CBRTF = @GNULIB_CBRTF@ GNULIB_CBRTL = @GNULIB_CBRTL@ GNULIB_CEIL = @GNULIB_CEIL@ GNULIB_CEILF = @GNULIB_CEILF@ GNULIB_CEILL = @GNULIB_CEILL@ GNULIB_CHDIR = @GNULIB_CHDIR@ GNULIB_CHOWN = @GNULIB_CHOWN@ GNULIB_CLOSE = @GNULIB_CLOSE@ GNULIB_COPYSIGN = @GNULIB_COPYSIGN@ GNULIB_COPYSIGNF = @GNULIB_COPYSIGNF@ GNULIB_COPYSIGNL = @GNULIB_COPYSIGNL@ GNULIB_COSF = @GNULIB_COSF@ GNULIB_COSHF = @GNULIB_COSHF@ GNULIB_COSL = @GNULIB_COSL@ GNULIB_DPRINTF = @GNULIB_DPRINTF@ GNULIB_DUP = @GNULIB_DUP@ GNULIB_DUP2 = @GNULIB_DUP2@ GNULIB_DUP3 = @GNULIB_DUP3@ GNULIB_DUPLOCALE = @GNULIB_DUPLOCALE@ GNULIB_ENVIRON = @GNULIB_ENVIRON@ GNULIB_EUIDACCESS = @GNULIB_EUIDACCESS@ GNULIB_EXP2 = @GNULIB_EXP2@ GNULIB_EXP2F = @GNULIB_EXP2F@ GNULIB_EXP2L = @GNULIB_EXP2L@ GNULIB_EXPF = @GNULIB_EXPF@ GNULIB_EXPL = @GNULIB_EXPL@ GNULIB_EXPM1 = @GNULIB_EXPM1@ GNULIB_EXPM1F = @GNULIB_EXPM1F@ GNULIB_EXPM1L = @GNULIB_EXPM1L@ GNULIB_FABSF = @GNULIB_FABSF@ GNULIB_FABSL = @GNULIB_FABSL@ GNULIB_FACCESSAT = @GNULIB_FACCESSAT@ GNULIB_FCHDIR = @GNULIB_FCHDIR@ GNULIB_FCHMODAT = @GNULIB_FCHMODAT@ GNULIB_FCHOWNAT = @GNULIB_FCHOWNAT@ GNULIB_FCLOSE = @GNULIB_FCLOSE@ GNULIB_FCNTL = @GNULIB_FCNTL@ GNULIB_FDATASYNC = @GNULIB_FDATASYNC@ GNULIB_FDOPEN = @GNULIB_FDOPEN@ GNULIB_FFLUSH = @GNULIB_FFLUSH@ GNULIB_FFS = @GNULIB_FFS@ GNULIB_FFSL = @GNULIB_FFSL@ GNULIB_FFSLL = @GNULIB_FFSLL@ GNULIB_FGETC = @GNULIB_FGETC@ GNULIB_FGETS = @GNULIB_FGETS@ GNULIB_FLOOR = @GNULIB_FLOOR@ GNULIB_FLOORF = @GNULIB_FLOORF@ GNULIB_FLOORL = @GNULIB_FLOORL@ GNULIB_FMA = @GNULIB_FMA@ GNULIB_FMAF = @GNULIB_FMAF@ GNULIB_FMAL = @GNULIB_FMAL@ GNULIB_FMOD = @GNULIB_FMOD@ GNULIB_FMODF = @GNULIB_FMODF@ GNULIB_FMODL = @GNULIB_FMODL@ GNULIB_FOPEN = @GNULIB_FOPEN@ GNULIB_FPRINTF = @GNULIB_FPRINTF@ GNULIB_FPRINTF_POSIX = @GNULIB_FPRINTF_POSIX@ GNULIB_FPURGE = @GNULIB_FPURGE@ GNULIB_FPUTC = @GNULIB_FPUTC@ GNULIB_FPUTS = @GNULIB_FPUTS@ GNULIB_FREAD = @GNULIB_FREAD@ GNULIB_FREOPEN = @GNULIB_FREOPEN@ GNULIB_FREXP = @GNULIB_FREXP@ GNULIB_FREXPF = @GNULIB_FREXPF@ GNULIB_FREXPL = @GNULIB_FREXPL@ GNULIB_FSCANF = @GNULIB_FSCANF@ GNULIB_FSEEK = @GNULIB_FSEEK@ GNULIB_FSEEKO = @GNULIB_FSEEKO@ GNULIB_FSTAT = @GNULIB_FSTAT@ GNULIB_FSTATAT = @GNULIB_FSTATAT@ GNULIB_FSYNC = @GNULIB_FSYNC@ GNULIB_FTELL = @GNULIB_FTELL@ GNULIB_FTELLO = @GNULIB_FTELLO@ GNULIB_FTRUNCATE = @GNULIB_FTRUNCATE@ GNULIB_FUTIMENS = @GNULIB_FUTIMENS@ GNULIB_FWRITE = @GNULIB_FWRITE@ GNULIB_GETC = @GNULIB_GETC@ GNULIB_GETCHAR = @GNULIB_GETCHAR@ GNULIB_GETCWD = @GNULIB_GETCWD@ GNULIB_GETDELIM = @GNULIB_GETDELIM@ GNULIB_GETDOMAINNAME = @GNULIB_GETDOMAINNAME@ GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = 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uninstall-am uninstall-binPROGRAMS uninstall-dist_sysconfDATA .PRECIOUS: Makefile # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: gnuastro-0.2.33-8a3b/bin/imgcrop/astimgcrop.conf0000644000175000017500000000200412601570666016351 00000000000000# Default parameters (System) for ImageCrop. # ImageCrop is part of GNU Astronomy Utitlies. # # Use the long option name of each paramter followed by # a value. The name and value should be separated by # atleast one of the following charaacters: # space, `,`, `=` or `:` # # Run with `--help` option or read the manual for a full # explanation of what each option means. # # NOTE I: All counting is from zero, not one. # NOTE II: Lines starting with `#` are ignored. # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Operating mode: imgmode 0 wcsmode 1 # Input image and catalog parameters: hdu 0 xcol 1 ycol 2 iwidth 201 racol 3 deccol 4 wwidth 3 hstartwcs 0 hendwcs 0 # Output parameters: checkcenter 3 suffix _crop.fits gnuastro-0.2.33-8a3b/bin/imgcrop/Makefile.am0000644000175000017500000000274112765246731015402 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. NOTE: $(top_srcdir)/bootstrapped/lib is only necessary ## for internally compiled utilities and libraries. It must not be included ## during the tests since the bootstrapped libraries are not installed. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Utility and its sources bin_PROGRAMS = astimgcrop astimgcrop_SOURCES = main.c main.h cite.h ui.c ui.h args.h imgcrop.c \ imgcrop.h wcsmode.c wcsmode.h crop.c crop.h astimgcrop_LDADD = $(top_builddir)/bootstrapped/lib/libgnu.la \ -lgnuastro ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.ma dist_sysconf_DATA = astimgcrop.conf gnuastro-0.2.33-8a3b/bin/header/0000755000175000017500000000000013004464724013201 500000000000000gnuastro-0.2.33-8a3b/bin/header/header.h0000644000175000017500000000205312616616510014522 00000000000000/********************************************************************* Header - View and manipulate a data file header Header is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef HEADER_H #define HEADER_H int header(struct headerparams *p); #endif gnuastro-0.2.33-8a3b/bin/header/header.c0000644000175000017500000001464112767351714014534 00000000000000/********************************************************************* Header - View and manipulate a data file header Header is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include "main.h" int haserror(struct headerparams *p, int actionid, char *string, int status) { char action[20]; int r=EXIT_SUCCESS; switch(actionid) { case 1: strcpy(action, "deleted"); break; case 2: strcpy(action, "renamed"); break; case 3: strcpy(action, "updated"); break; case 4: strcpy(action, "written"); break; default: error(EXIT_FAILURE, 0, "a bug! Please contact us at `%s' so we can fix " "this problem. In `header.c'. The value of actionid in " "`haserror' must not be %d", PACKAGE_BUGREPORT, actionid); } if(p->quitonerror) { fits_report_error(stderr, status); error(EXIT_FAILURE, 0, "not deleted: %s\n", string); } else { fprintf(stderr, "Not deleted: %s\n", string); r=EXIT_FAILURE; } return r; } void writeupdatekeys(fitsfile *fptr, struct gal_fits_key_ll **keylist, int u1w2) { int status=0; struct gal_fits_key_ll *tmp, *ttmp; tmp=*keylist; while(tmp!=NULL) { /* Write the information: */ if(u1w2==1) { if(tmp->value) { if( fits_update_key(fptr, tmp->datatype, tmp->keyname, tmp->value, tmp->comment, &status) ) gal_fits_io_error(status, NULL); } else { if(fits_write_key_null(fptr, tmp->keyname, tmp->comment, &status)) gal_fits_io_error(status, NULL); } } else if (u1w2==2) { if(tmp->value) { if( fits_write_key(fptr, tmp->datatype, tmp->keyname, tmp->value, tmp->comment, &status) ) gal_fits_io_error(status, NULL); } else { if(fits_write_key_null(fptr, tmp->keyname, tmp->comment, &status)) gal_fits_io_error(status, NULL); } if(tmp->unit && fits_write_key_unit(fptr, tmp->keyname, tmp->unit, &status) ) gal_fits_io_error(status, NULL); } else error(EXIT_FAILURE, 0, "a bug! Please contact us at `%s' so we can " "fix this problem. In `header.c'. The value of u1w2 in " "writeupdatekeys must not be %d\n", PACKAGE_BUGREPORT, u1w2); /* Add the unit: */ if(tmp->unit && fits_write_key_unit(fptr, tmp->keyname, tmp->unit, &status) ) gal_fits_io_error(status, NULL); /* Free the value pointer if desired: */ if(tmp->kfree) free(tmp->keyname); if(tmp->vfree) free(tmp->value); if(tmp->cfree) free(tmp->comment); /* Keep the pointer to the next keyword and free the allocated space for this keyword.*/ ttmp=tmp->next; free(tmp); tmp=ttmp; } *keylist=NULL; } int header(struct headerparams *p) { size_t i=0; int r=EXIT_SUCCESS; int nkeys, status=0; char *fullheader, *c, *cf; struct gal_linkedlist_stll *tstll, *ttstll; if(p->onlyview) { if( fits_hdr2str(p->fptr, 0, NULL, 0, &fullheader, &nkeys, &status) ) gal_fits_io_error(status, NULL); /* FLEN_CARD supposes that the NULL string character is in the end of each keyword header card. In fits_hdr2str, the NULL characters are removed and so the maximum length is one less. */ cf=(c=fullheader)+nkeys*(FLEN_CARD-1); do { if(i && i%(FLEN_CARD-1)==0) putc('\n', stdout); putc(*c++, stdout); ++i; } while(cdelete) { for(tstll=p->delete; tstll!=NULL; tstll=tstll->next) { fits_delete_key(p->fptr, tstll->v, &status); if(status) r=haserror(p, 1, tstll->v, status); } } if(p->up.rename) { ttstll=p->renameto; for(tstll=p->renamefrom; tstll!=NULL; tstll=tstll->next) { fits_modify_name(p->fptr, tstll->v, ttstll->v, &status); if(status) r=haserror(p, 2, tstll->v, status); ttstll=ttstll->next; } } if(p->update) writeupdatekeys(p->fptr, &p->update, 1); if(p->write) writeupdatekeys(p->fptr, &p->write, 2); if(p->asis) for(tstll=p->asis; tstll!=NULL; tstll=tstll->next) { fits_write_record(p->fptr, tstll->v, &status); if(status) r=haserror(p, 1, tstll->v, status); } if(p->history) { fits_write_history(p->fptr, p->history, &status); if(status) r=haserror(p, 4, "HISTORY", status); } if(p->comment) { fits_write_comment(p->fptr, p->comment, &status); if(status) r=haserror(p, 4, "COMMENT", status); } if(p->date) { fits_write_date(p->fptr, &status); if(status) r=haserror(p, 4, "DATE", status); } } return r; } gnuastro-0.2.33-8a3b/bin/header/args.h0000644000175000017500000001436312774160421014235 00000000000000/********************************************************************* Header - View and manipulate a data file header Header is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef ARGS_H #define ARGS_H #include #include #include #include /**************************************************************/ /************** argp.h definitions ***************/ /**************************************************************/ /* Definition parameters for the argp: */ const char *argp_program_version=SPACK_STRING"\n"GAL_STRINGS_COPYRIGHT "\n\nWritten by Mohammad Akhlaghi"; const char *argp_program_bug_address=PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata"; const char doc[] = /* Before the list of options: */ GAL_STRINGS_TOP_HELP_INFO SPACK_NAME" print the header information in any astronomical data file" "header. It can also manipulate (add, remove or modify) any of the " "existing keywords in a data header. \n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /* Available letters for short options: b e f g i j k l m n p s v x y z A B C E F G I J L M O R T U W X Y Z Number keys used: Nothing! Options with keys (second structure element) larger than 500 do not have a short version. */ static struct argp_option options[] = { { 0, 0, 0, 0, "Input:", 1 }, { 0, 0, 0, 0, "Output:", 2 }, { "asis", 'a', "STR", 0, "Write the argument string as is into the header.", 2 }, { "delete", 'd', "STR", 0, "Delete a keyword from the header.", 2 }, { "rename", 'r', "STR", 0, "Rename keyword, keeping value and comments.", 2 }, { "update", 'u', "STR", 0, "Update a keyword value or comments.", 2 }, { "write", 'w', "STR", 0, "Write a keyword (with value, comments and units).", 2 }, { "history", 'H', "STR", 0, "Add HISTORY keyword, any length is ok.", 2 }, { "comment", 'c', "STR", 0, "Add COMMENT keyword, any length is ok.", 2 }, { "date", 't', 0, 0, "Set the DATE keyword to the current time.", 2 }, { 0, 0, 0, 0, "Operating modes:", -1 }, { "quitonerror", 'Q', 0, 0, "Quit if there is an error on any action.", -1 }, {0} }; /* Parse a single option: */ static error_t parse_opt(int key, char *arg, struct argp_state *state) { /* Save the arguments structure: */ struct headerparams *p = state->input; /* Set the pointer to the common parameters for all programs here: */ state->child_inputs[0]=&p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); switch(key) { /* Input: */ /* Output: */ case 'a': gal_linkedlist_add_to_stll(&p->asis, arg); break; case 'd': gal_linkedlist_add_to_stll(&p->delete, arg); break; case 'r': gal_linkedlist_add_to_stll(&p->up.rename, arg); break; case 'u': gal_linkedlist_add_to_stll(&p->up.update, arg); break; case 'w': gal_linkedlist_add_to_stll(&p->up.write, arg); break; case 'c': p->comment=arg; break; case 'H': p->history=arg; break; case 't': p->date=1; break; /* Operating modes: */ case 'Q': p->quitonerror=1; /* Read the non-option arguments: */ case ARGP_KEY_ARG: /* See what type of input value it is and put it in. */ if( gal_fits_name_is_fits(arg) ) { if(p->up.inputname) argp_error(state, "only one input image should be given"); else p->up.inputname=arg; } else argp_error(state, "%s is not a valid file type", arg); break; /* The command line options and arguments are finished. */ case ARGP_KEY_END: if(p->cp.setdirconf==0 && p->cp.setusrconf==0 && p->cp.printparams==0) { if(state->arg_num==0) argp_error(state, "no argument given"); if(p->up.inputname==NULL) argp_error(state, "no input FITS image(s) provided"); } break; default: return ARGP_ERR_UNKNOWN; } return 0; } /* Specify the children parsers: */ struct argp_child children[]= { {&commonargp, 0, NULL, 0}, {0, 0, 0, 0} }; /* Basic structure defining the whole argument reading process. */ static struct argp thisargp = {options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif gnuastro-0.2.33-8a3b/bin/header/ui.h0000644000175000017500000000215412722534072013711 00000000000000/********************************************************************* Header - View and manipulate a data file header Header is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef UI_H #define UI_H void setparams(int argc, char *argv[], struct headerparams *p); void freeandreport(struct headerparams *p); #endif gnuastro-0.2.33-8a3b/bin/header/ui.c0000644000175000017500000002771113001632537013706 00000000000000/********************************************************************* Header - View and manipulate a data file header Header is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include /* From Gnulib. */ #include /* Includes time.h and sys/time.h */ #include #include #include #include "main.h" #include "ui.h" /* Needs main.h */ #include "args.h" /* Needs main.h, includes argp.h. */ /* Set the file names of the places where the default parameters are put. */ #define CONFIG_FILE SPACK CONF_POSTFIX #define SYSCONFIG_FILE SYSCONFIG_DIR "/" CONFIG_FILE #define USERCONFIG_FILEEND USERCONFIG_DIR CONFIG_FILE #define CURDIRCONFIG_FILE CURDIRCONFIG_DIR CONFIG_FILE /**************************************************************/ /************** Options and parameters ***************/ /**************************************************************/ void readconfig(char *filename, struct headerparams *p) { FILE *fp; size_t lineno=0, len=200; char *line, *name, *value; /*struct uiparams *up=&p->up;*/ struct gal_commonparams *cp=&p->cp; char key='a'; /* Not used, just a place holder. */ /* When the file doesn't exist or can't be opened, it is ignored. It might be intentional, so there is no error. If a parameter is missing, it will be reported after all defaults are read. */ fp=fopen(filename, "r"); if (fp==NULL) return; /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); /* Read the tokens in the file: */ while(getline(&line, &len, fp) != -1) { /* Prepare the "name" and "value" strings, also set lineno. */ GAL_CONFIGFILES_START_READING_LINE; /* Inputs: */ if(strcmp(name, "hdu")==0) gal_checkset_allocate_copy_set(value, &cp->hdu, &cp->hduset); /* Outputs */ /* Operating modes: */ /* Read options common to all programs */ GAL_CONFIGFILES_READ_COMMONOPTIONS_FROM_CONF else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s` not recognized.\n", name); } free(line); fclose(fp); } void printvalues(FILE *fp, struct headerparams *p) { /*struct uiparams *up=&p->up;*/ struct gal_commonparams *cp=&p->cp; /* Print all the options that are set. Separate each group with a commented line explaining the options in that group. */ fprintf(fp, "\n# Input image:\n"); if(cp->hduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("hdu", cp->hdu); /* For the operating mode, first put the macro to print the common options, then the (possible options particular to this program). */ fprintf(fp, "\n# Operating mode:\n"); GAL_CONFIGFILES_PRINT_COMMONOPTIONS; } /* Note that numthreads will be used automatically based on the configure time. */ void checkifset(struct headerparams *p) { /*struct uiparams *up=&p->up;*/ struct gal_commonparams *cp=&p->cp; int intro=0; if(cp->hduset==0) GAL_CONFIGFILES_REPORT_NOTSET("hdu"); GAL_CONFIGFILES_END_OF_NOTSET_REPORT; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ void sanitycheck(struct headerparams *p) { if(p->delete || p->up.update || p->up.write || p->asis || p->comment || p->history || p->date || p->up.rename) p->onlyview=0; else p->onlyview=1; } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ void setuprename(struct headerparams *p) { char *c; struct gal_linkedlist_stll *tmp; for(tmp=p->up.rename; tmp!=NULL; tmp=tmp->next) { /* `c' is created in case of an error, so the input value can be reported. */ errno=0; c=malloc(strlen(tmp->v) + 1); if(c==NULL) error(EXIT_FAILURE, errno, "space for c in setuprename"); strcpy(c, tmp->v); /* Tokenize the input. */ gal_linkedlist_add_to_stll(&p->renamefrom, strtok(tmp->v, ", ")); gal_linkedlist_add_to_stll(&p->renameto, strtok(NULL, ", ")); if(p->renamefrom->v==NULL || p->renameto->v==NULL) error(EXIT_FAILURE, 0, "`%s' could not be tokenized in order to " "complete rename. There should be a space character " "or a comma (,) between the two keyword names. If you have " "used the space character, be sure to enclose the value to " "the `--rename' option in double quotation marks", c); free(c); } /* { struct gal_linkedlist_stll *tmp2=p->renameto; for(tmp=p->renamefrom; tmp!=NULL; tmp=tmp->next) { printf("%s to %s\n", tmp->v, tmp2->v); tmp2=tmp2->next; } } */ } void fillfitsheaderll(struct gal_linkedlist_stll *input, struct gal_fits_key_ll **output) { long l, *lp; void *fvalue; double d, *dp; struct gal_linkedlist_stll *tmp; int i=0, datatype, vfree; char *c, *cf, *start, *tailptr; char *original, *keyname, *value, *comment, *unit; for(tmp=input; tmp!=NULL; tmp=tmp->next) { i=0; tailptr=NULL; /* `c' is created in case of an error, so the input value can be reported. */ errno=0; original=malloc(strlen(tmp->v)+1); if(original==NULL) error(EXIT_FAILURE, errno, "space for c in setuprename"); strcpy(original, tmp->v); /* Tokenize the input. Note that strlen does not include the \0 character. So we have added it with a 1. */ cf=(c=start=tmp->v)+strlen(tmp->v)+1; keyname=value=comment=unit=NULL; do { switch(*c) { case ',': case '\0': *c='\0'; if(start!=c) switch(i) { case 0: keyname=start; break; case 1: value=start; break; case 2: comment=start; break; case 3: unit=start; break; default: error(EXIT_FAILURE, 0, "%s: only three commas should " "be given in the write or update keyword " "options. The general expected format is:\n" " KEYWORD,value,\"a comment string\",unit\n", original); } ++i; start=c+1; break; default: break; } } while(++cup.inputname)+strlen(p->cp.hdu)+4; ffname=malloc(len*sizeof *ffname); if(ffname==NULL) error(EXIT_FAILURE, errno, "%zu characters", len); sprintf(ffname, "%s[%s#]", p->up.inputname, p->cp.hdu); /* Open the FITS file: */ if(p->onlyview) iomode=READONLY; else iomode=READWRITE; if( fits_open_file(&p->fptr, ffname, iomode, &status) ) gal_fits_io_error(status, "reading file"); free(ffname); /* Separate the comma-separated values: */ if(p->up.rename) setuprename(p); if(p->up.update) fillfitsheaderll(p->up.update, &p->update); if(p->up.write) fillfitsheaderll(p->up.write, &p->write); } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void setparams(int argc, char *argv[], struct headerparams *p) { struct gal_commonparams *cp=&p->cp; /* Set the non-zero initial values, the structure was initialized to have a zero value for all elements. */ cp->spack = SPACK; cp->verb = 1; cp->numthreads = num_processors(NPROC_CURRENT); cp->removedirinfo = 1; /* Read the arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Add the user default values and save them if asked. */ GAL_CONFIGFILES_CHECK_SET_CONFIG; /* Check if all the required parameters are set. */ checkifset(p); /* Print the values for each parameter. */ if(cp->printparams) GAL_CONFIGFILES_REPORT_PARAMETERS_SET; /* Do a sanity check. */ sanitycheck(p); /* Make the array of input images. */ preparearrays(p); } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void freeandreport(struct headerparams *p) { int status=0; /* Free the allocated arrays: */ free(p->cp.hdu); free(p->cp.output); /* Close the FITS file: */ if(fits_close_file(p->fptr, &status)) gal_fits_io_error(status, NULL); if(p->wcs) wcsvfree(&p->nwcs, &p->wcs); } gnuastro-0.2.33-8a3b/bin/header/cite.h0000644000175000017500000000316012750745735014231 00000000000000/********************************************************************* Header - View and manipulate a data file header Header is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CITE_H #define CITE_H #define HEADERBIBTEX "" #define PRINTCITEABORT { \ printf("\nWe hope %s has been useful for your research.\n" \ "Citations are vital for the continued work on %s.\n" \ "Thank you for citing it in your research paper.\n" \ "\nPlease cite as \"%s\":\n\n%s\n\n%s", \ SPACK_NAME, SPACK_NAME, SPACK_STRING, \ GAL_STRINGS_MAIN_BIBTEX, HEADERBIBTEX); \ exit(EXIT_SUCCESS); \ } #endif gnuastro-0.2.33-8a3b/bin/header/main.h0000644000175000017500000000570112774156524014232 00000000000000/********************************************************************* Header - View and manipulate a data file header Header is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include #include /* Progarm name macros: */ #define SPACK "astheader" /* Subpackage executable name. */ #define SPACK_NAME "Header" /* Subpackage full name. */ #define SPACK_STRING SPACK_NAME" ("PACKAGE_NAME") "PACKAGE_VERSION struct uiparams { char *inputname; /* Name of input file. */ struct gal_linkedlist_stll *rename; /* Rename a keyword. */ struct gal_linkedlist_stll *update; /* For keywords to update. */ struct gal_linkedlist_stll *write; /* Full arg. for keywords to add. */ }; struct headerparams { /* Other structures: */ struct uiparams up; /* User interface parameters. */ struct gal_commonparams cp; /* Common parameters. */ /* Input: */ int nwcs; /* Number of WCS structures. */ fitsfile *fptr; /* FITS file pointer. */ struct wcsprm *wcs; /* Pointer to WCS structures. */ /* Output: */ int date; /* Set DATE to current time. */ char *comment; /* COMMENT value. */ char *history; /* HISTORY value. */ struct gal_linkedlist_stll *asis; /* Strings to write as is into header.*/ struct gal_linkedlist_stll *delete; /* Keywords to remove. */ struct gal_linkedlist_stll *renamefrom; /* The initial value of the keyword. */ struct gal_linkedlist_stll *renameto; /* The final value of the keyword. */ struct gal_fits_key_ll *update; /* Linked list of keywords to update. */ struct gal_fits_key_ll *write; /* Linked list of keywords to add. */ /* Operating mode: */ int quitonerror; /* Quit if an error occurs. */ /* Internal: */ int onlyview; time_t rawtime; /* Starting time of the program. */ }; #endif gnuastro-0.2.33-8a3b/bin/header/main.c0000644000175000017500000000312012774156733014220 00000000000000/********************************************************************* Header - View and manipulate a data file header Header is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include /* Includes time.h and sys/time.h */ #include "main.h" #include "ui.h" /* needs main.h. */ #include "header.h" /* needs main.h. */ int main (int argc, char *argv[]) { int r; struct headerparams p={{0}, {0}, 0}; /* Get the starting time. */ time(&p.rawtime); /* Read the input parameters. */ setparams(argc, argv, &p); /* Run MakeProfiles */ r=header(&p); /* Free all non-freed allocations. */ freeandreport(&p); /* Return successfully.*/ return r; } gnuastro-0.2.33-8a3b/bin/header/Makefile.in0000644000175000017500000017246713004464626015210 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is 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= @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ 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.NOEXPORT: gnuastro-0.2.33-8a3b/bin/header/astheader.conf0000644000175000017500000000134012510547112015720 00000000000000# Default parameters (System) for Header. # Header is part of GNU Astronomy Utitlies. # # Use the long option name of each paramter followed by # a value. The name and value should be separated by # atleast one of the following charaacters: # space, `,`, `=` or `:` # # Run with `--help` option or read the manual for a full # explanation of what each option means. # # NOTE I: All counting is from zero, not one. # NOTE II: Lines starting with `#` are ignored. # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Input: hdu 0 # Output:gnuastro-0.2.33-8a3b/bin/header/Makefile.am0000644000175000017500000000267212765246732015176 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. NOTE: $(top_srcdir)/bootstrapped/lib is only necessary ## for internally compiled utilities and libraries. It must not be included ## during the tests since the bootstrapped libraries are not installed. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Utility and its sources bin_PROGRAMS = astheader astheader_SOURCES = main.c main.h cite.h ui.c ui.h args.h \ header.c header.h astheader_LDADD = $(top_builddir)/bootstrapped/lib/libgnu.la \ -lgnuastro ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astheader.conf gnuastro-0.2.33-8a3b/bin/cosmiccal/0000755000175000017500000000000013004464724013706 500000000000000gnuastro-0.2.33-8a3b/bin/cosmiccal/cosmiccal.h0000644000175000017500000000241712722534072015740 00000000000000/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef COSMICCAL_H #define COSMICCAL_H /* For the GSL integrations */ #define GSLILIMIT 1000 #define GSLIEPSABS 0 #define GSLIEPSREL 1e-7 /* Format of final outputs */ # define FLTFORMAT " - %-55s%f\n" # define EXPFORMAT " - %-55s%e\n" void cosmiccal(struct cosmiccalparams *p); #endif gnuastro-0.2.33-8a3b/bin/cosmiccal/cosmiccal.c0000644000175000017500000001622112722534072015731 00000000000000/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include "main.h" #include "cosmiccal.h" /**************************************************************/ /************ Integrand functions *************/ /**************************************************************/ /* In these functions, z as a separate argument, this is not necessarily the same z as the redshift in cosmiccalparams. */ double Ez(double z, void *params) { struct cosmiccalparams *p=(struct cosmiccalparams *)params; return sqrt( p->olambda + p->ocurv * (1+z) * (1+z) + p->omatter * (1+z) * (1+z) * (1+z) + p->oradiation * (1+z) * (1+z) * (1+z) * (1+z)); } double age(double z, void *params) { return 1 / ( (1+z)*Ez(z,params) ); } double propdist(double z, void *params) { return 1 / ( Ez(z,params) ); } /**************************************************************/ /************ Integrators *************/ /**************************************************************/ /* Estimate the age of the universe, note that z might be different from the desired redshift. */ double ageofuniverse(struct cosmiccalparams *p, double z) { gsl_function F; double result, error; gsl_integration_workspace *w=gsl_integration_workspace_alloc(GSLILIMIT); /* Set the GSL function parameters */ F.params=p; F.function=&age; gsl_integration_qagiu(&F, z, GSLIEPSABS, GSLIEPSREL, GSLILIMIT, w, &result, &error); return result / p->H0s / (365*GSL_CONST_MKSA_DAY) / 1e9; } /* Return the proper distance to a source at z in units of mega parsecs */ double properdistance(struct cosmiccalparams *p, double z) { size_t neval; gsl_function F; double result, error; /* Set the GSL function parameters */ F.params=p; F.function=&propdist; gsl_integration_qng(&F, 0.0f, z, GSLIEPSABS, GSLIEPSREL, &result, &error, &neval); return result * p->c / p->H0s / (1e6 * GSL_CONST_MKSA_PARSEC); } double covolume(double z, void *params) { size_t neval; gsl_function F; double result, error; /* Set the GSL function parameters */ F.params=params; F.function=&propdist; gsl_integration_qng(&F, 0.0f, z, GSLIEPSABS, GSLIEPSREL, &result, &error, &neval); return result * result / ( Ez(z,params) ); } double comovingvolume(struct cosmiccalparams *p, double z) { size_t neval; gsl_function F; double result, error; double cH = p->c / p->H0s / (1e6 * GSL_CONST_MKSA_PARSEC); /* Set the GSL function parameters */ F.params=p; F.function=&covolume; gsl_integration_qng(&F, 0.0f, z, GSLIEPSABS, GSLIEPSREL, &result, &error, &neval); return result * 4 * M_PI * cH*cH*cH; } /**************************************************************/ /************ Intermediary functions *************/ /**************************************************************/ /* Critical density at redshift z in units of gram/cm^3*/ double criticaldensity(struct cosmiccalparams *p, double z) { double H = p->H0s*Ez(z,p); return 3*H*H/(8*M_PI*GSL_CONST_MKSA_GRAVITATIONAL_CONSTANT)/1000; } /**************************************************************/ /************ Main function *************/ /**************************************************************/ void cosmiccal(struct cosmiccalparams *p) { double ad, ld, vz, pd, absmagconv; double curage, ccritd, distmod, outage, zcritd; /* In case the user just wants one number, only print that and return. */ if(p->onlyvolume){ printf("%f\n", comovingvolume(p,p->redshift)); return; } if(p->onlyabsmagconv){ pd=properdistance(p, p->redshift); ld=pd*(1+p->redshift); distmod=5*(log10(ld*1000000)-1); absmagconv=distmod-2.5*log10(1+p->redshift); printf("%f\n", absmagconv); return; } /* The user wants everything, do all the calculations and print everything with full descriptions. */ curage=ageofuniverse(p, 0.0f); ccritd=criticaldensity(p, 0.0f); vz=comovingvolume(p,p->redshift); pd=properdistance(p, p->redshift); outage=ageofuniverse(p, p->redshift); zcritd=criticaldensity(p, p->redshift); ad=pd/(1+p->redshift); ld=pd*(1+p->redshift); distmod=5*(log10(ld*1000000)-1); absmagconv=distmod-2.5*log10(1+p->redshift); /* Print out results: */ printf("%s\n", SPACK_STRING); printf("\n Input parameters\n"); printf( " ----------------\n"); printf(FLTFORMAT, "Desired redshift for calculations (z):", p->redshift); printf(FLTFORMAT, "Expansion rate (Hubble constant, H0), now:", p->H0); printf(FLTFORMAT, "Cosmological constant fractional density, now:", p->olambda); printf(FLTFORMAT, "Matter fractional density, now:", p->omatter); printf(EXPFORMAT, "Radiation fractional density, now:", p->oradiation); printf(EXPFORMAT, "Curvatue fractional density (from the above):", p->ocurv); printf("\n\n Universe now\n"); printf( " ------------\n"); printf(FLTFORMAT, "Age of Universe now (Gyr):", curage); printf(EXPFORMAT, "Critical density now (g/cm^3):", ccritd); printf(FLTFORMAT, "Proper distance to z (Mpc):", pd); printf(FLTFORMAT, "Angular diameter distance to z (Mpc):", ad); printf(FLTFORMAT, "Tangential distance covered by 1 arcsec at z (Kpc):", ad*1000*M_PI/3600/180); printf(FLTFORMAT, "Luminosity distance to z (Mpc):", ld); printf(FLTFORMAT, "Distance modulus at z (no unit):", distmod); printf(FLTFORMAT, "Conversion to absolute magnitude (no unit):", absmagconv); printf("\n\n Universe at desired redshift z\n"); printf( " ------------------------------\n"); printf(FLTFORMAT, "Age of Universe at z (Gyr):", outage); printf(FLTFORMAT, "Look-back time to z (Gyr):", curage-outage); printf(EXPFORMAT, "Critical density at z (g/cm^3):", zcritd); printf("\n\n Comoving universe (time independent)\n"); printf( " ------------------------------------\n"); printf(FLTFORMAT, "Comoving volume over 4pi stradian to z (Mpc^3):", vz); } gnuastro-0.2.33-8a3b/bin/cosmiccal/args.h0000644000175000017500000001425512774157077014757 00000000000000/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef ARGS_H #define ARGS_H #include #include #include #include /**************************************************************/ /************** argp.h definitions ***************/ /**************************************************************/ /* Definition parameters for the argp: */ const char *argp_program_version=SPACK_STRING"\n"GAL_STRINGS_COPYRIGHT "\n\nWritten by Mohammad Akhlaghi"; const char *argp_program_bug_address=PACKAGE_BUGREPORT; static char args_doc[] = ""; const char doc[] = /* Before the list of options: */ GAL_STRINGS_TOP_HELP_INFO SPACK_NAME" will produce cosmological calculations.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /* Available letters for short options: b c d e f g i j k m n p s t u w x y A B C E F G I J L M O Q R T U W X Y Z Number keys used: <=500 Options with keys (second structure element) larger than 500 do not have a short version. */ static struct argp_option options[] = { { 0, 0, 0, 0, "Input:", 1 }, { "redshift", 'z', "FLT", 0, "Redshift of interest.", 1 }, { "H0", 'H', "FLT", 0, "Current expansion rate (Hubble constant).", 1 }, { "olambda", 'l', "FLT", 0, "Current cosmological cst. dens. per crit. dens.", 1 }, { "omatter", 'm', "FLT", 0, "Current matter density per critical density.", 1 }, { "oradiation", 'r', "FLT", 0, "Current radiation density per critical density.", 1 }, { 0, 0, 0, 0, "Output:", 2 }, { "onlyvolume", 'v', 0, 0, "Only print comoving volume in Mpc^3", 2 }, { "onlyabsmagconv", 'a', 0, 0, "Only print conversion to absolute magnitude.", 2 }, { 0, 0, 0, 0, "Operating modes:", -1 }, {0} }; /* Parse a single option: */ static error_t parse_opt(int key, char *arg, struct argp_state *state) { /* Save the arguments structure: */ struct cosmiccalparams *p = state->input; /* Set the pointer to the common parameters for all programs here: */ state->child_inputs[0]=&p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); switch(key) { /* Input: */ case 'z': gal_checkset_double_el_0(arg, &p->redshift, "redshift", key, SPACK, NULL, 0); p->up.redshiftset=1; break; case 'H': gal_checkset_double_el_0(arg, &p->H0, "H0", key, SPACK, NULL, 0); p->up.H0set=1; break; case 'l': gal_checkset_double_el_0(arg, &p->olambda, "olambda", key, SPACK, NULL, 0); p->up.olambdaset=1; break; case 'm': gal_checkset_double_el_0(arg, &p->omatter, "omatter", key, SPACK, NULL, 0); p->up.omatterset=1; break; case 'r': gal_checkset_double_el_0(arg, &p->oradiation, "oradiation", key, SPACK, NULL, 0); p->up.oradiationset=1; break; /* Output: */ case 'v': p->onlyvolume=1; p->up.onlyvolumeset=1; break; case 'a': p->onlyabsmagconv=1; p->up.onlyabsmagconvset=1; break; /* Operating modes: */ /* Read the non-option arguments: */ case ARGP_KEY_ARG: argp_error(state, SPACK_NAME" only takes options as " "input, currently no arguments are supported"); break; /* The command line options and arguments are finished. */ case ARGP_KEY_END: /* Currently there are no arguments, or input files, so there is no need for such checks. if(p->cp.setdirconf==0 && p->cp.setusrconf==0 && p->cp.printparams==0) { if(state->arg_num==0) argp_error(state, "no argument given"); if(p->up.inputname==NULL) argp_error(state, "no input FITS image(s) provided"); } */ break; default: return ARGP_ERR_UNKNOWN; } return 0; } /* Specify the children parsers: */ struct argp_child children[]= { {&commonargp, 0, NULL, 0}, {0, 0, 0, 0} }; /* Basic structure defining the whole argument reading process. */ static struct argp thisargp = {options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif gnuastro-0.2.33-8a3b/bin/cosmiccal/ui.h0000644000175000017500000000212112722534072014410 00000000000000/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef UI_H #define UI_H void setparams(int argc, char *argv[], struct cosmiccalparams *p); #endif gnuastro-0.2.33-8a3b/bin/cosmiccal/ui.c0000644000175000017500000002210513002762710014401 00000000000000/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include /* From Gnulib. */ #include #include #include #include /* Includes time.h and sys/time.h */ #include #include #include #include "main.h" #include "ui.h" /* Needs main.h */ #include "args.h" /* Needs main.h, includes argp.h. */ /* Set the file names of the places where the default parameters are put. */ #define CONFIG_FILE SPACK CONF_POSTFIX #define SYSCONFIG_FILE SYSCONFIG_DIR "/" CONFIG_FILE #define USERCONFIG_FILEEND USERCONFIG_DIR CONFIG_FILE #define CURDIRCONFIG_FILE CURDIRCONFIG_DIR CONFIG_FILE /**************************************************************/ /************** Options and parameters ***************/ /**************************************************************/ void readconfig(char *filename, struct cosmiccalparams *p) { FILE *fp; size_t lineno=0, len=200; char *line, *name, *value; struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; char key='a'; /* Not used, just a place holder. */ /* When the file doesn't exist or can't be opened, it is ignored. It might be intentional, so there is no error. If a parameter is missing, it will be reported after all defaults are read. */ fp=fopen(filename, "r"); if (fp==NULL) return; /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); /* Read the tokens in the file: */ while(getline(&line, &len, fp) != -1) { /* Prepare the "name" and "value" strings, also set lineno. */ GAL_CONFIGFILES_START_READING_LINE; /* Inputs: */ if(strcmp(name, "redshift")==0) { if(up->redshiftset) continue; gal_checkset_double_el_0(value, &p->redshift, name, key, SPACK, filename, lineno); up->redshiftset=1; } else if(strcmp(name, "H0")==0) { if(up->H0set) continue; gal_checkset_double_el_0(value, &p->H0, name, key, SPACK, filename, lineno); up->H0set=1; } else if(strcmp(name, "olambda")==0) { if(up->olambdaset) continue; gal_checkset_double_el_0(value, &p->olambda, name, key, SPACK, filename, lineno); up->olambdaset=1; } else if(strcmp(name, "omatter")==0) { if(up->omatterset) continue; gal_checkset_double_el_0(value, &p->omatter, name, key, SPACK, filename, lineno); up->omatterset=1; } else if(strcmp(name, "oradiation")==0) { if(up->oradiationset) continue; gal_checkset_double_el_0(value, &p->oradiation, name, key, SPACK, filename, lineno); up->oradiationset=1; } /* Outputs */ else if(strcmp(name, "onlyvolume")==0) { if(up->onlyvolumeset) continue; gal_checkset_int_zero_or_one(value, &p->onlyvolume, name, key, SPACK, filename, lineno); up->onlyvolumeset=1; } else if(strcmp(name, "onlyabsmagconv")==0) { if(up->onlyabsmagconvset) continue; gal_checkset_int_zero_or_one(value, &p->onlyabsmagconv, name, key, SPACK, filename, lineno); up->onlyabsmagconvset=1; } /* Operating modes: */ /* Read options common to all programs */ GAL_CONFIGFILES_READ_COMMONOPTIONS_FROM_CONF else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s` not recognized.\n", name); } free(line); fclose(fp); } void printvalues(FILE *fp, struct cosmiccalparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; /* Print all the options that are set. Separate each group with a commented line explaining the options in that group. */ fprintf(fp, "\n# Input:\n"); if(up->redshiftset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "redshift", p->redshift); if(up->H0set) fprintf(fp, CONF_SHOWFMT"%.3f\n", "H0", p->H0); fprintf(fp, "\n# Current densities per current critical density:\n"); if(up->olambdaset) fprintf(fp, CONF_SHOWFMT"%.5f\n", "olambda", p->olambda); if(up->omatterset) fprintf(fp, CONF_SHOWFMT"%.5f\n", "omatter", p->omatter); if(up->oradiationset) fprintf(fp, CONF_SHOWFMT"%.5f\n", "oradiation", p->oradiation); /* For the operating mode, first put the macro to print the common options, then the (possible options particular to this program). */ fprintf(fp, "\n# Operating mode:\n"); GAL_CONFIGFILES_PRINT_COMMONOPTIONS; } /* Note that numthreads will be used automatically based on the configure time. */ void checkifset(struct cosmiccalparams *p) { struct uiparams *up=&p->up; /*struct gal_commonparams *cp=&p->cp;*/ int intro=0; if(up->redshiftset==0) GAL_CONFIGFILES_REPORT_NOTSET("redshift"); if(up->H0set==0) GAL_CONFIGFILES_REPORT_NOTSET("H0"); if(up->olambdaset==0) GAL_CONFIGFILES_REPORT_NOTSET("olambda"); if(up->omatterset==0) GAL_CONFIGFILES_REPORT_NOTSET("omatter"); if(up->oradiationset==0) GAL_CONFIGFILES_REPORT_NOTSET("oradiation"); GAL_CONFIGFILES_END_OF_NOTSET_REPORT; } /**************************************************************/ /************ Sanity check *************/ /**************************************************************/ void sanitycheck(struct cosmiccalparams *p) { int check=p->onlyvolume+p->onlyabsmagconv; /* If only one of the single output options are called, then check should be 1, if none are called, then it should be zero. However, if more than one is called, check will be larger than one. So in this case, report an error. */ if(check>1) error(EXIT_FAILURE, 0, "only a single option starting with `--only' " "can be called"); } /**************************************************************/ /************ Preparations *************/ /**************************************************************/ void preparations(struct cosmiccalparams *p) { /* Speed of light: */ p->c=GSL_CONST_MKSA_SPEED_OF_LIGHT; /* The curvature fractional density: */ p->ocurv=1-(p->olambda+p->omatter+p->oradiation); /* Convert H0 from km/sec/Mpc to 1/sec: */ p->H0s=p->H0/1000/GSL_CONST_MKSA_PARSEC; } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void setparams(int argc, char *argv[], struct cosmiccalparams *p) { struct gal_commonparams *cp=&p->cp; /* Set the non-zero initial values, the structure was initialized to have a zero value for all elements. */ cp->spack = SPACK; cp->verb = 1; cp->numthreads = num_processors(NPROC_CURRENT); cp->removedirinfo = 1; /* Read the arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Add the user default values and save them if asked. */ GAL_CONFIGFILES_CHECK_SET_CONFIG; /* Check if all the required parameters are set. */ checkifset(p); /* Do a sanity check */ sanitycheck(p); /* Make the preparations */ preparations(p); /* Print the values for each parameter. */ if(cp->printparams) GAL_CONFIGFILES_REPORT_PARAMETERS_SET; } gnuastro-0.2.33-8a3b/bin/cosmiccal/cite.h0000644000175000017500000000320012750745735014731 00000000000000/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CITE_H #define CITE_H #define COSMICCALBIBTEX "" #define PRINTCITEABORT { \ printf("\nWe hope %s has been useful for your research.\n" \ "Citations are vital for the continued work on %s.\n" \ "Thank you for citing it in your research paper.\n" \ "\nPlease cite as \"%s\":\n\n%s\n\n%s", \ SPACK_NAME, SPACK_NAME, SPACK_STRING, \ GAL_STRINGS_MAIN_BIBTEX, COSMICCALBIBTEX); \ exit(EXIT_SUCCESS); \ } #endif gnuastro-0.2.33-8a3b/bin/cosmiccal/main.h0000644000175000017500000000544212774156733014743 00000000000000/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include /* Progarm name macros: */ #define SPACK "astcosmiccal" /* Subpackage executable name. */ #define SPACK_NAME "CosmicCalculator" /* Subpackage full name. */ #define SPACK_STRING SPACK_NAME" ("PACKAGE_NAME") "PACKAGE_VERSION struct uiparams { int redshiftset; int curvatureset; int H0set; int olambdaset; int omatterset; int oradiationset; int onlyvolumeset; int onlyabsmagconvset; }; struct cosmiccalparams { /* Other structures: */ struct uiparams up; /* User interface parameters. */ struct gal_commonparams cp; /* Common parameters. */ /* Input: */ double redshift; /* Redshift of interest. */ double H0; /* Current expansion rate (km/sec/Mpc). */ double olambda; /* Current cosmological constant dens. */ double omatter; /* Current matter density. */ double oradiation; /* Current radiation density. */ double solidangle; /* Solid angle for volume (in stradian).*/ /* Output: */ int onlyvolume; /* Only print the volume in Mpc^3. */ int onlyabsmagconv; /* Only print conversion to abs. mag. */ /* Operating mode: */ /* Internal: */ double K; /* Curvature constant. */ double c; /* Speed of light. */ double H0s; /* Current expansion rate (1/sec). */ double ocurv; /* Curvature density today. */ time_t rawtime; /* Starting time of the program. */ }; #endif gnuastro-0.2.33-8a3b/bin/cosmiccal/main.c0000644000175000017500000000304712774156734014736 00000000000000/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include /* Includes time.h and sys/time.h */ #include "main.h" #include "ui.h" /* needs main.h. */ #include "cosmiccal.h" /* needs main.h. */ int main (int argc, char *argv[]) { struct cosmiccalparams p={{0}, {0}, 0}; /* Get the starting time. */ time(&p.rawtime); /* Read the input parameters. */ setparams(argc, argv, &p); /* Run MakeProfiles */ cosmiccal(&p); /* Return successfully.*/ return EXIT_SUCCESS; } gnuastro-0.2.33-8a3b/bin/cosmiccal/Makefile.in0000644000175000017500000017260613004464626015710 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # This program is distributed in 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GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ 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limit (for SysV at least) may be exceeded. .NOEXPORT: gnuastro-0.2.33-8a3b/bin/cosmiccal/astcosmiccal.conf0000644000175000017500000000240112772147615017147 00000000000000# Default parameters (System) for CosmicCalculator. # CosmicCalculator is part of GNU Astronomy Utitlies. # # Use the long option name of each paramter followed by # a value. The name and value should be separated by # atleast one of the following charaacters: # space, `,`, `=` or `:` # # Run with `--help` option or read the manual for a full # explanation of what each option means. # # NOTE I: All counting is from zero, not one. # NOTE II: Lines starting with `#` are ignored. # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Citation # ======== # # The current default cosmological values in CosmicCalculator are taken # from the Planck 2015 results (paper XIII, A&A 594, A13 (2016), Table 4, # page 31, last column: "TT,TE,EE+lowP+lensing+ext"). # # http://www.aanda.org/articles/aa/full_html/2016/10/aa25830-15/aa25830-15.html # # IMPORTANT NOTES: If you change these system-wide default values, please # change this comment and cite the source. # Input: redshift 1 H0 67.74 olambda 0.6911 omatter 0.3089 oradiation 0.0 # Output: gnuastro-0.2.33-8a3b/bin/cosmiccal/Makefile.am0000644000175000017500000000271412765246732015700 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2016, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. NOTE: $(top_srcdir)/bootstrapped/lib is only necessary ## for internally compiled utilities and libraries. It must not be included ## during the tests since the bootstrapped libraries are not installed. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Utility and its sources bin_PROGRAMS = astcosmiccal astcosmiccal_SOURCES = main.c main.h cite.h ui.c ui.h args.h \ cosmiccal.c cosmiccal.h astcosmiccal_LDADD = $(top_builddir)/bootstrapped/lib/libgnu.la \ -lgnuastro ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astcosmiccal.conf gnuastro-0.2.33-8a3b/bin/convolve/0000755000175000017500000000000013004464724013604 500000000000000gnuastro-0.2.33-8a3b/bin/convolve/cite.h0000644000175000017500000000316712750745735014643 00000000000000/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see .x **********************************************************************/ #ifndef CITE_H #define CITE_H #define CONVOLVEBIBTEX "" #define PRINTCITEABORT { \ printf("\nWe hope %s has been useful for your research.\n" \ "Citations are vital for the continued work on %s.\n" \ "Thank you for citing it in your research paper.\n" \ "\nPlease cite as \"%s\":\n\n%s\n\n%s", \ SPACK_NAME, SPACK_NAME, SPACK_STRING, \ GAL_STRINGS_MAIN_BIBTEX, CONVOLVEBIBTEX); \ exit(EXIT_SUCCESS); \ } #endif gnuastro-0.2.33-8a3b/bin/convolve/convolve.h0000644000175000017500000000346412764767045015555 00000000000000/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CONVOLVE_H #define CONVOLVE_H #include struct fftonthreadparams { /* Operating info: */ size_t id; /* The number of this thread. */ struct convolveparams *p; /* Pointer to main program structure. */ int forward1backwardn1; /* Operate on one or two images. */ size_t stride; /* 1D FFT on rows or columns? */ /* Pointers to GSL FFT structures: */ gsl_fft_complex_wavetable *ps0wave; gsl_fft_complex_wavetable *ps1wave; gsl_fft_complex_workspace *ps0work; gsl_fft_complex_workspace *ps1work; /* Thread parameters. */ size_t *indexs; /* Indexs to be used in this thread. */ pthread_barrier_t *b; /* Barrier to keep threads waiting. */ }; void convolve(struct convolveparams *p); #endif gnuastro-0.2.33-8a3b/bin/convolve/convolve.c0000644000175000017500000005556513001632537015537 00000000000000/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include "main.h" #include "convolve.h" /******************************************************************/ /************* Complex numbers *****************/ /******************************************************************/ /* We have a complex (R+iI) array and we want to display it. But we can only do that either with the spectrum, or the phase: Spectrum: sqrt(R^2+I^2) Phase: arctan(I/R) */ void complextoreal(double *c, size_t size, int action, double **output) { double *out, *o, *of; errno=0; *output=out=malloc(size*sizeof *out); if(out==NULL) error(EXIT_FAILURE, errno, "%zu bytes for out in complextoreal", size*sizeof *out); of=(o=out)+size; switch(action) { case COMPLEXTOREALSPEC: do { *o++ = sqrt( *c**c + *(c+1)**(c+1) ); c+=2; } while(oMINGOODDIVSPEC) { r = ( ( (*a * *b) + (*(a+1) * *(b+1)) ) / ( *b * *b + *(b+1) * *(b+1) ) ); *(a+1) = ( ( (*(a+1) * *b) - (*a * *(b+1)) ) / ( *b * *b + *(b+1) * *(b+1) ) ); *a=r; if(sqrt(*a**a + *(a+1)**(a+1))>1.00001f) *a=*(a+1)=0.0f; } else { *a=0; *(a+1)=0; } a+=2; b+=2; } while(ainput, *kernel=p->kernel; size_t is0=p->is0, is1=p->is1, ks0=p->ks0, ks1=p->ks1; /* Find the sizes of the padded image, note that since the kernel sizes are always odd, the extra padding on the input image is always going to be an even number (clearly divisable). */ ps0=p->ps0 = p->makekernel ? p->is0 : p->is0+p->ks0-1; ps1=p->ps1 = p->makekernel ? p->is1 : p->is1+p->ks1-1; /* The Discrete Fourier transforms operate faster on even-sized arrays. So if the padded sides are not even, make them so: */ if(ps0%2) ps0=p->ps0=ps0+1; if(ps1%2) ps1=p->ps1=ps1+1; /* Allocate the space for the padded input image and fill it. */ errno=0; pimg=p->pimg=malloc(2*ps0*ps1*sizeof *pimg); if(pimg==NULL) error(EXIT_FAILURE, errno, "%zu bytes for pimg", 2*ps0*ps1*sizeof *pimg); for(i=0;ipker=malloc(2*ps0*ps1*sizeof *pker); if(pker==NULL) error(EXIT_FAILURE, errno, "%zu bytes for pker", 2*ps0*ps1*sizeof *pker); for(i=0;iks0-1. Since p->ks0 is always odd, the padding will alwys be even. */ void removepaddingcorrectroundoff(struct convolveparams *p) { size_t ps1=p->ps1; float *o, *input=p->input; size_t i, hi0, hi1, is0, is1; double *d, *df, *start, *pimg=p->pimg; /* Set all the necessary parameters to crop the desired region. hi0 and hi1 are the coordinates of the first pixel in the output image. In the case of deconvolution, if the maximum radius is larger smaller than the input image, we will also only be using region that contains non-zero rows and columns.*/ if(p->makekernel) { hi0 = 2*p->makekernel-1is0 ? p->ps0/2-p->makekernel : 0; hi1 = 2*p->makekernel-1is1 ? p->ps1/2-p->makekernel : 0; p->is0 = 2*p->makekernel-1is0 ? 2*p->makekernel-1 : p->is0; p->is1 = 2*p->makekernel-1is1 ? 2*p->makekernel-1 : p->is1; } else { hi0=(p->ks0-1)/2; hi1=(p->ks1-1)/2; } is0=p->is0; is1=p->is1; /* To start with, `start' points to the first pixel in the final image: */ start=&pimg[hi0*ps1+hi1]; for(i=0;iCONVFLOATINGPOINTERR ) ? *d : 0.0f; while (++dcp.numthreads*sizeof *fp); if(fp==NULL) error(EXIT_FAILURE, errno, "%zu bytes in forward2dfft for fp", p->cp.numthreads*sizeof *fp); /* Initialize the gsl_fft_wavetable structures (these are thread safe): */ fp[0].ps0wave=gsl_fft_complex_wavetable_alloc(p->ps0); fp[0].ps1wave=gsl_fft_complex_wavetable_alloc(p->ps1); /* Set the values for all the other threads: */ for(i=0;icp.numthreads;++i) { fp[i].p=p; fp[i].ps0wave=fp[0].ps0wave; fp[i].ps1wave=fp[0].ps1wave; fp[i].ps0work=gsl_fft_complex_workspace_alloc(p->ps0); fp[i].ps1work=gsl_fft_complex_workspace_alloc(p->ps1); } } void freefp(struct fftonthreadparams *fp) { size_t i; gsl_fft_complex_wavetable_free(fp[0].ps0wave); gsl_fft_complex_wavetable_free(fp[0].ps1wave); for(i=0;ip->cp.numthreads;++i) { gsl_fft_complex_workspace_free(fp[i].ps0work); gsl_fft_complex_workspace_free(fp[i].ps1work); } free(fp); } /* Unfortunately I don't understand why the division operation in deconvolution (makekernel) does not produce a centered image, the image is translated by half the input size in both dimensions. So I am correcting this in the spatial domain here. */ void correctdeconvolve(struct convolveparams *p, double **spatial) { double r, *s, *n, *d, *df, sum=0.0f; size_t i, j, ps0=p->ps0, ps1=p->ps1; int ii, jj, ci=p->ps0/2-1, cj=p->ps1/2-1; /* Check if the image has even sides. */ if(ps0%2 || ps1%2) error(EXIT_FAILURE, 0, "a bug! Please contact us at %s. In " "correctdeconvolve, the padded image sides are not an " "even number", PACKAGE_BUGREPORT); /* First convert the complex image to a real image: */ complextoreal(p->pimg, ps0*ps1, COMPLEXTOREALSPEC, &s); /* Allocate the array to keep the new values */ errno=0; n=malloc(ps0*ps1*sizeof *n); if(n==NULL) error(EXIT_FAILURE, errno, "%zu bytes for n in correctdeconvolve " "(convolve.c). ", ps0*ps1*sizeof *n); /* Put the elements in their proper place: For example in one dimention where the values are actually the true distances: s[0]=0, s[1]=1, s[2]=2, s[3]=3, s[4]=4, s[5]=5 We want the value 0 to be in the `center'. Note that `s' is periodic, for example the next 6 elements have distances: s[6]=0, s[7]=1, s[8]=2, s[9]=3, s[10]=4, s[11]=5 So a `center'ed array would be like: s[0]=4, s[1]=5, s[2]=0, s[3]=1, s[4]=2, s[5]=3 The relations between the old (i and j) and new (ii and jj) come from something like the above line. */ for(i=0;ips0/2 ? i-(ps0/2+1) : i+ps0/2-1; for(j=0;jps1/2 ? j-(ps1/2+1) : j+ps1/2-1; r=sqrt( (ii-ci)*(ii-ci) + (jj-cj)*(jj-cj) ); sum += n[ii*ps1+jj] = r < p->makekernel ? s[i*ps1+j] : 0; /*printf("(%zu, %zu) --> (%zu, %zu)\n", i, j, ii, jj);*/ } } /* Divide all elements by the sum so the kernel is normalized: */ df=(d=n)+ps0*ps1; do *d++/=sum; while(ds0 and p->s1. When there are two images, then the index numbers are going to be at most double p->s0 and p->s1. In this case, those index values which are smaller than p->s0 or p->s1 belong to the input image and those which are equal or larger than larger belong to the kernel image (after subtraction for p->s0 or p->s1).*/ void * onedimensionfft(void *inparam) { struct fftonthreadparams *fp = (struct fftonthreadparams *)inparam; struct convolveparams *p=fp->p; double *d, *df; size_t indmultip, maxindex; gsl_fft_complex_workspace *work; gsl_fft_complex_wavetable *wavetable; double *data, *pimg=p->pimg, *pker=p->pker; int forward1backwardn1=fp->forward1backwardn1; size_t i, size, stride=fp->stride, *indexs=fp->indexs; /* Set the number of points to transform, indmultip: The value to be multiplied by the value in indexs to specify the first pixel of the row or column. */ if(stride==1) { size=p->ps1; wavetable=fp->ps1wave; work=fp->ps1work; maxindex=p->ps0; indmultip=p->ps1; } else { size=p->ps0; wavetable=fp->ps0wave; work=fp->ps0work; maxindex=p->ps1; indmultip=1; } /* Go over all the rows or columns given for this thread. NOTE: The final array (after the two FFT'd arrays are multiplied by each other) is stored in p->pimg. So the check below works both in the forward and the backward transformation. */ for(i=0;indexs[i]!=GAL_THREADS_NON_THRD_INDEX;++i) { data = ( indexs[i]cp.numthreads>1) pthread_barrier_wait(fp->b); return NULL; } /* Do the forward Fast Fourier Transform either on two input images (the padded image and kernel) or on one image (the multiplication of the FFT of the two). In the second case, it is assumed that we are looking at the complex conjugate of the array so in practice this will be a backward transform. */ void twodimensionfft(struct convolveparams *p, struct fftonthreadparams *fp, int forward1backwardn1) { int err; pthread_t t; /* All thread ids saved in this, not used. */ pthread_attr_t attr; pthread_barrier_t b; size_t i, nb, *indexs, thrdcols; size_t nt=p->cp.numthreads, multiple=0; /* First we are going to get the 1D fourier transform on the rows of both images. */ if(forward1backwardn1==1) multiple=2; else if(forward1backwardn1==-1) multiple=1; else error(EXIT_FAILURE, 0, "a bug! In forward2dfft, the value of the " "variable forward1backwardn1 is somehow not 1 or 2, but %d. " "Please contact us at "PACKAGE_BUGREPORT" so we can find the " "cause of the problem and fix it", forward1backwardn1); /* ==================== */ /* 1D FFT on each row. */ /* ==================== */ gal_threads_dist_in_threads(multiple*p->ps0, nt, &indexs, &thrdcols); if(nt==1) { fp[0].stride=1; fp[0].indexs=&indexs[0]; fp[0].forward1backwardn1=forward1backwardn1; onedimensionfft(&fp[0]); } else { /* Initialize the attributes. Note that this running thread (that spinns off the nt threads) is also a thread, so the number the barrier should be one more than the number of threads spinned off. */ if( multiple*p->ps0 < nt ) nb=multiple*p->ps0+1; else nb=nt+1; gal_threads_attr_barrier_init(&attr, &b, nb); /* Spin off the threads: */ for(i=0;ips1s! */ gal_threads_dist_in_threads(multiple*p->ps1, nt, &indexs, &thrdcols); if(nt==1) { fp[0].stride=p->ps1; fp[0].indexs=indexs; fp[0].forward1backwardn1=forward1backwardn1; onedimensionfft(&fp[0]); } else { if( multiple*p->ps1 < nt ) nb=multiple*p->ps1+1; else nb=nt+1; gal_threads_attr_barrier_init(&attr, &b, nb); for(i=0;ips1; /* On each column, stride is p->ps1 */ fp[i].indexs=&indexs[i*thrdcols]; fp[i].forward1backwardn1=forward1backwardn1; err=pthread_create(&t, &attr, onedimensionfft, &fp[i]); if(err) error(EXIT_FAILURE, 0, "can't create thread %zu for columns", i); } pthread_barrier_wait(&b); pthread_attr_destroy(&attr); pthread_barrier_destroy(&b); } free(indexs); } void frequencyconvolve(struct convolveparams *p) { double *tmp; struct timeval t1; int verb=p->cp.verb; struct fftonthreadparams *fp; char *operation = p->makekernel ? "Divided" : "Multiplied"; /* Make the padded arrays. */ if(verb) gettimeofday(&t1, NULL); makepaddedcomplex(p); if(verb) gal_timing_report(&t1, "Input and Kernel images padded.", 1); if(p->viewfreqsteps) { complextoreal(p->pimg, p->ps0*p->ps1, COMPLEXTOREALREAL, &tmp); gal_fits_array_to_file(p->up.freqstepsname, "Input padded", DOUBLE_IMG, tmp, p->ps0, p->ps1, 0, NULL, NULL, SPACK_STRING); free(tmp); complextoreal(p->pker, p->ps0*p->ps1, COMPLEXTOREALREAL, &tmp); gal_fits_array_to_file(p->up.freqstepsname, "Kernel padded", DOUBLE_IMG, tmp, p->ps0, p->ps1, 0, NULL, NULL, SPACK_STRING); free(tmp); } /* Initialize the structures: */ fftinitializer(p, &fp); /* Forward 2D FFT on each image. */ if(verb) gettimeofday(&t1, NULL); twodimensionfft(p, fp, 1); if(verb) gal_timing_report(&t1, "Images converted to frequency domain.", 1); if(p->viewfreqsteps) { complextoreal(p->pimg, p->ps0*p->ps1, COMPLEXTOREALSPEC, &tmp); gal_fits_array_to_file(p->up.freqstepsname, "Input transform", DOUBLE_IMG, tmp, p->ps0, p->ps1, 0, NULL, NULL, SPACK_STRING); free(tmp); complextoreal(p->pker, p->ps0*p->ps1, COMPLEXTOREALSPEC, &tmp); gal_fits_array_to_file(p->up.freqstepsname, "Kernel transform", DOUBLE_IMG, tmp, p->ps0, p->ps1, 0, NULL, NULL, SPACK_STRING); free(tmp); } /* Multiply or divide the two arrays and save them in the output.*/ if(verb) gettimeofday(&t1, NULL); if(p->makekernel) { complexarraydivide(p->pimg, p->pker, p->ps0*p->ps1); if(verb) gal_timing_report(&t1, "Divided in the frequency domain.", 1); } else { complexarraymultiply(p->pimg, p->pker, p->ps0*p->ps1); if(verb) gal_timing_report(&t1, "Multiplied in the frequency domain.", 1); } if(p->viewfreqsteps) { complextoreal(p->pimg, p->ps0*p->ps1, COMPLEXTOREALSPEC, &tmp); gal_fits_array_to_file(p->up.freqstepsname, operation, DOUBLE_IMG, tmp, p->ps0, p->ps1, 0, NULL, NULL, SPACK_STRING); free(tmp); } /* Forward (in practice inverse) 2D FFT on each image. */ if(verb) gettimeofday(&t1, NULL); twodimensionfft(p, fp, -1); if(p->makekernel) correctdeconvolve(p, &tmp); else complextoreal(p->pimg, p->ps0*p->ps1, COMPLEXTOREALREAL, &tmp); if(verb) gal_timing_report(&t1, "Converted back to the spatial domain.", 1); if(p->viewfreqsteps) { gal_fits_array_to_file(p->up.freqstepsname, "Spatial", DOUBLE_IMG, tmp, p->ps0, p->ps1, 0, NULL, NULL, SPACK_STRING); free(tmp); } /* Free the padded arrays (they are no longer needed) and put the converted array (that is real, not complex) in p->pimg. */ free(p->pimg); free(p->pker); p->pimg=tmp; /* Crop out the center, numbers smaller than 10^{-17} are errors, remove them. */ if(verb) gettimeofday(&t1, NULL); removepaddingcorrectroundoff(p); if(verb) gal_timing_report(&t1, "Padded parts removed.", 1); /* Free all the allocated space. */ freefp(fp); } /******************************************************************/ /************* Outside function *****************/ /******************************************************************/ void convolve(struct convolveparams *p) { float *convolved; long *meshindexs; struct gal_mesh_params *mp=&p->mp; /* Do the convolution. */ if(p->spatial) { /* Prepare the mesh structure: */ mp->img=p->input; mp->s0=p->is0; mp->s1=p->is1; mp->kernel=p->kernel; mp->ks0=p->ks0; mp->ks1=p->ks1; mp->numthreads=p->cp.numthreads; gal_mesh_make_mesh(mp); if(p->meshname) { gal_mesh_check_mesh_id(mp, &meshindexs); gal_fits_array_to_file(p->meshname, "Input", FLOAT_IMG, p->mp.img, mp->s0, mp->s1, p->anyblank, p->wcs, NULL, SPACK_STRING); gal_fits_array_to_file(p->meshname, "MeshIndexs", LONG_IMG, meshindexs, mp->s0, mp->s1, 0, p->wcs, NULL, SPACK_STRING); free(meshindexs); } /* Do the spatial convolution on the mesh: */ gal_mesh_spatial_convolve_on_mesh(mp, &convolved); /* Replace the input image array with the convolved array: */ free(p->input); p->input=convolved; } else frequencyconvolve(p); /* Save the output (which is in p->input) array. Note that p->input will be freed in ui.c. */ gal_fits_array_to_file(p->cp.output, "Convolved", FLOAT_IMG, p->input, p->is0, p->is1, p->anyblank, p->wcs, NULL, SPACK_STRING); } gnuastro-0.2.33-8a3b/bin/convolve/ui.h0000644000175000017500000000221212616616510014307 00000000000000/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef UI_H #define UI_H void setparams(int argc, char *argv[], struct convolveparams *p); void freeandreport(struct convolveparams *p, struct timeval *t1); #endif gnuastro-0.2.33-8a3b/bin/convolve/ui.c0000644000175000017500000004576513001632537014322 00000000000000/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* From Gnulib. */ #include #include #include #include /* Includes time.h and sys/time.h */ #include #include #include "main.h" #include "ui.h" /* Needs main.h. */ #include "args.h" /* Needs main.h, includes argp.h. */ /* Set the file names of the places where the default parameters are put. */ #define CONFIG_FILE SPACK CONF_POSTFIX #define SYSCONFIG_FILE SYSCONFIG_DIR "/" CONFIG_FILE #define USERCONFIG_FILEEND USERCONFIG_DIR CONFIG_FILE #define CURDIRCONFIG_FILE CURDIRCONFIG_DIR CONFIG_FILE /**************************************************************/ /************** Options and parameters ***************/ /**************************************************************/ void readconfig(char *filename, struct convolveparams *p) { FILE *fp; size_t lineno=0, len=200; char *line, *name, *value; struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; int zeroorone, spatialset=0, frequencyset=0; char key='a'; /* Not used, just a place holder. */ /* When the file doesn't exist or can't be opened, it is ignored. It might be intentional, so there is no error. If a parameter is missing, it will be reported after all defaults are read. */ fp=fopen(filename, "r"); if (fp==NULL) return; /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); /* Read the tokens in the file: */ while(getline(&line, &len, fp) != -1) { /* Prepare the "name" and "value" strings, also set lineno. */ GAL_CONFIGFILES_START_READING_LINE; /* Inputs: */ if(strcmp(name, "hdu")==0) gal_checkset_allocate_copy_set(value, &cp->hdu, &cp->hduset); else if (strcmp(name, "mask")==0) gal_checkset_allocate_copy_set(value, &up->maskname, &up->masknameset); else if (strcmp(name, "mhdu")==0) gal_checkset_allocate_copy_set(value, &up->mhdu, &up->mhduset); else if (strcmp(name, "kernel")==0) gal_checkset_allocate_copy_set(value, &up->kernelname, &up->kernelnameset); else if (strcmp(name, "khdu")==0) gal_checkset_allocate_copy_set(value, &up->khdu, &up->khduset); /* Outputs: */ else if(strcmp(name, "output")==0) gal_checkset_allocate_copy_set(value, &cp->output, &cp->outputset); /* Mesh grid: */ else if(strcmp(name, "meshsize")==0) { if(up->meshsizeset) continue; gal_checkset_sizet_l_zero(value, &p->mp.meshsize, name, key, SPACK, filename, lineno); up->meshsizeset=1; } else if(strcmp(name, "nch1")==0) { if(up->nch1set) continue; gal_checkset_sizet_l_zero(value, &p->mp.nch1, name, key, SPACK, filename, lineno); up->nch1set=1; } else if(strcmp(name, "nch2")==0) { if(up->nch2set) continue; gal_checkset_sizet_l_zero(value, &p->mp.nch2, name, key, SPACK, filename, lineno); up->nch2set=1; } else if(strcmp(name, "lastmeshfrac")==0) { if(up->lastmeshfracset) continue; gal_checkset_float_l_0_s_1(value, &p->mp.lastmeshfrac, name, key, SPACK, filename, lineno); up->lastmeshfracset=1; } else if(strcmp(name, "fullconvolution")==0) { if(up->fullconvolutionset) continue; gal_checkset_int_zero_or_one(value, &p->mp.fullconvolution, name, key, SPACK, filename, lineno); up->fullconvolutionset=1; } /* Operating modes: */ else if(strcmp(name, "spatial")==0) { gal_checkset_int_zero_or_one(value, &zeroorone, name, key, SPACK, filename, lineno); if(zeroorone) { spatialset=1; if(frequencyset) error_at_line(EXIT_FAILURE, 0, filename, lineno, "Spatial and frequency modes cannot be called " "together. It is ambiguous."); if(up->spatialset==0) { p->spatial=1; p->frequency=0; up->spatialset=up->frequencyset=1; } } } else if(strcmp(name, "frequency")==0) { gal_checkset_int_zero_or_one(value, &zeroorone, name, key, SPACK, filename, lineno); if(zeroorone) { frequencyset=1; if(spatialset) error_at_line(EXIT_FAILURE, 0, filename, lineno, "Spatial and frequency modes cannot be " "called together. It is ambiguous."); if(up->frequencyset==0) { p->spatial=0; p->frequency=1; up->spatialset=up->frequencyset=1; } } } else if(strcmp(name, "makekernel")==0) { if(up->makekernelset) continue; gal_checkset_int_el_zero(value, &p->makekernel, name, key, SPACK, filename, lineno); up->makekernelset=1; } /* Read options common to all programs */ GAL_CONFIGFILES_READ_COMMONOPTIONS_FROM_CONF else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s` not recognized.\n", name); } free(line); fclose(fp); } void printvalues(FILE *fp, struct convolveparams *p) { struct uiparams *up=&p->up; struct gal_mesh_params *mp=&p->mp; struct gal_commonparams *cp=&p->cp; fprintf(fp, "\n# Input:\n"); if(cp->hduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("hdu", cp->hdu); if(up->masknameset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("mask", up->maskname); if(up->mhduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("mhdu", up->mhdu); if(up->kernelnameset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("kernel", up->kernelname); if(up->khduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("khdu", up->khdu); fprintf(fp, "\n# Output:\n"); if(cp->outputset) fprintf(fp, CONF_SHOWFMT"%s\n", "output", cp->output); fprintf(fp, "\n# Mesh grid:\n"); if(up->meshsizeset) fprintf(fp, CONF_SHOWFMT"%zu\n", "meshsize", mp->meshsize); if(up->nch1set) fprintf(fp, CONF_SHOWFMT"%zu\n", "nch1", mp->nch1); if(up->nch2set) fprintf(fp, CONF_SHOWFMT"%zu\n", "nch2", mp->nch2); if(up->lastmeshfracset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "lastmeshfrac", mp->lastmeshfrac); if(up->fullconvolutionset) fprintf(fp, CONF_SHOWFMT"%d\n", "fullconvolution", mp->fullconvolution); /* For the operating mode, first put the macro to print the common options, then the (possible options particular to this program). */ fprintf(fp, "\n# Operating modes:\n"); GAL_CONFIGFILES_PRINT_COMMONOPTIONS; if(up->spatialset) fprintf(fp, CONF_SHOWFMT"%d\n", "spatial", p->spatial); if(up->frequencyset) fprintf(fp, CONF_SHOWFMT"%d\n", "frequency", p->frequency); if(up->makekernelset) fprintf(fp, CONF_SHOWFMT"%d\n", "makekernel", p->makekernel); } void checkifset(struct convolveparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; int intro=0; /* Input: */ if(cp->hduset==0) GAL_CONFIGFILES_REPORT_NOTSET("hdu"); if(up->kernelnameset==0) GAL_CONFIGFILES_REPORT_NOTSET("kernel"); if(up->khduset==0) GAL_CONFIGFILES_REPORT_NOTSET("khdu"); /* Mesh grid: */ if(up->meshsizeset==0) GAL_CONFIGFILES_REPORT_NOTSET("meshsize"); if(up->nch1set==0) GAL_CONFIGFILES_REPORT_NOTSET("nch1"); if(up->nch2set==0) GAL_CONFIGFILES_REPORT_NOTSET("nch2"); if(up->lastmeshfracset==0) GAL_CONFIGFILES_REPORT_NOTSET("lastmeshfrac"); if(up->fullconvolutionset==0) GAL_CONFIGFILES_REPORT_NOTSET("fullconvolution"); /* Operating mode: */ if(up->spatialset==0 && up->frequencyset==0) GAL_CONFIGFILES_REPORT_NOTSET("spatial or frequency"); if(up->makekernelset==0) GAL_CONFIGFILES_REPORT_NOTSET("makekernel"); GAL_CONFIGFILES_END_OF_NOTSET_REPORT; } /**************************************************************/ /************ Prepare the arrays *************/ /**************************************************************/ void sanitycheck(struct convolveparams *p) { char *outsuffix = p->makekernel ? "_kernel.fits" : "_convolved.fits"; /* Make sure the input file exists. */ gal_checkset_check_file(p->up.inputname); /* Set maskname accordingly: */ gal_fits_file_or_ext_name(p->up.inputname, p->cp.hdu, p->up.masknameset, &p->up.maskname, p->up.mhdu, p->up.mhduset, "mask"); /* Check the output file name: */ if(p->cp.outputset) { if( gal_checkset_dir_0_file_1(p->cp.output, p->cp.dontdelete) == 0 ) error(EXIT_FAILURE, 0, "your output name (%s) is a directory", p->cp.output); } else { gal_checkset_automatic_output(p->up.inputname, outsuffix, p->cp.removedirinfo, p->cp.dontdelete, &p->cp.output); p->cp.outputset=1; } if(p->frequency && p->viewfreqsteps) gal_checkset_automatic_output(p->up.inputname, "_freqsteps.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->up.freqstepsname); /* Check output names: */ if(p->meshname) { p->meshname=NULL; /* Was not allocated before! */ gal_checkset_automatic_output(p->up.inputname, "_mesh.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->meshname); } /* makekernel can only operate in frequency mode: */ if(p->makekernel && p->spatial) error(EXIT_FAILURE, 0, "`--makekernel' (`-m') can only be defined " "in frequency domain operations, not spatial domain. You can " "either explicitly call for frequency mode on the command line " "or change your nearest configuration file so Convolve defaults " "to the frequency domain. Please see the Gnuastro for more " "information. On the command line, the manual can be seen with " "the `info gnuastro' command"); } /**************************************************************/ /************ Prepare the arrays *************/ /**************************************************************/ void preparearrays(struct convolveparams *p) { size_t i, size; int bitpix, anyblank; struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; float *f, *fp, tmp, *kernel, sum; /* First read the input image: */ gal_fits_file_to_float(up->inputname, up->maskname, cp->hdu, up->mhdu, &p->input, &bitpix, &p->anyblank, &p->is0, &p->is1); gal_fits_read_wcs(up->inputname, cp->hdu, 0, 0, &p->nwcs, &p->wcs); if(p->frequency && p->anyblank) fprintf(stderr, "\n----------------------------------------\n" "######## %s WARNING ########\n" "There are blank (masked) pixels in %s (hdu: %s) and you " "have asked for frequency domain convolution.%s All the " "convolved pixels will become blank. Only spatial domain " "convolution can account for blank (masked) pixels in the " "input data.\n" "----------------------------------------\n\n", SPACK_NAME, up->inputname, cp->hdu, up->maskname ? "" : " Even though you have not provided any mask image, " "these are the blank pixels in the input image, see the `Blank " "pixels' section of the Gnuastro manual for more information."); /* Read the file specified by --kernel. If makekernel is specified, then this is actually the low resolution image. */ if(p->makekernel) { /* Read in the kernel array: */ gal_fits_file_to_float(up->kernelname, NULL, up->khdu, NULL, &p->kernel, &bitpix, &anyblank, &p->ks0, &p->ks1); if(p->ks0!=p->is0 || p->ks1!=p->is1) error(EXIT_FAILURE, 0, "with the `--makekernel' (`-m') option, " "the input image and the image specified with the kernel " "option should have the same size. The lower resolution " "input image (%s) has %zux%zu pixels while the higher " "resolution image (%s) specified with the kernel option has " "%zux%zu pixels", up->inputname, p->is1, p->is0, up->kernelname, p->ks1, p->ks0); /* Divide both images by their sum so their lowest frequency becomes 1 (and their division would be meaningful!).*/ size=p->is0*p->is1; sum=gal_statistics_float_sum(p->input, size); gal_array_fmultip_const(p->input, size, 1/sum); sum=gal_statistics_float_sum(p->kernel, size); gal_array_fmultip_const(p->kernel, size, 1/sum); } /* Read the kernel. If there is anything particular to Convolve, then don't use the standard kernel reading function in fits.c. Otherwise just use the same one that all programs use. The standard one is faster because it mixes the NaN conversion and also the normalization into one loop.*/ else { if(p->kernelnorm==0 || p->kernelflip==0) { /* Read in the kernel array: */ gal_fits_file_to_float(up->kernelname, NULL, up->khdu, NULL, &p->kernel, &bitpix, &anyblank, &p->ks0, &p->ks1); size=p->ks0*p->ks1; kernel=p->kernel; if(p->ks0%2==0 || p->ks1%2==0) error(EXIT_FAILURE, 0, "the kernel image has to have an odd " "number of pixels on both sides (there has to be on pixel " "in the center). %s (hdu: %s) is %zu by %zu", p->up.kernelname, p->up.khdu, p->ks1, p->ks0); /* Convert all the NaN pixels to zero if the kernel contains blank pixels. */ if(anyblank) { fp=(f=kernel)+size; do if(isnan(*f)) *f=0.0f; while(++fkernelnorm) { sum=gal_statistics_float_sum(kernel, size); gal_array_fmultip_const(kernel, size, 1/sum); } /* Flip the kernel: */ if(p->spatial && p->kernelflip) for(i=0;ikernelname, up->khdu, &p->kernel, &p->ks0, &p->ks1); } } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void setparams(int argc, char *argv[], struct convolveparams *p) { struct gal_commonparams *cp=&p->cp; /* Set the non-zero initial values, the structure was initialized to have a zero value for all elements. */ cp->spack = SPACK; cp->verb = 1; cp->numthreads = num_processors(NPROC_CURRENT); cp->removedirinfo = 1; /* Set non-zero options: */ p->kernelflip = 1; p->kernelnorm = 1; /* Read the arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Add the user default values and save them if asked. */ GAL_CONFIGFILES_CHECK_SET_CONFIG; /* Check if all the required parameters are set. */ checkifset(p); /* Print the values for each parameter. */ if(cp->printparams) GAL_CONFIGFILES_REPORT_PARAMETERS_SET; /* Do a sanity check, then remove the possibly existing log file created by gal_txtarray_txt_to_array. */ sanitycheck(p); /* Prepare the necessary arrays: */ preparearrays(p); /* Everything is ready, notify the user of the program starting. */ if(cp->verb) { printf(SPACK_NAME" started on %s", ctime(&p->rawtime)); printf(" - Using %zu CPU threads.\n", p->cp.numthreads); printf(" - Input: %s (hdu: %s)\n", p->up.inputname, p->cp.hdu); if(p->up.maskname) printf(" - Mask: %s (hdu: %s)\n", p->up.maskname, p->up.mhdu); printf(" - Kernel: %s (hdu: %s)\n", p->up.kernelname, p->up.khdu); } } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void freeandreport(struct convolveparams *p, struct timeval *t1) { free(p->input); free(p->kernel); free(p->cp.hdu); free(p->up.khdu); free(p->meshname); free(p->cp.output); wcsvfree(&p->nwcs, &p->wcs); /* Free the mask image name. Note that p->up.inputname was not allocated, but given to the program by the operating system. */ if(p->up.maskname && p->up.maskname!=p->up.inputname) free(p->up.maskname); /* Print the final message. */ if(p->cp.verb) gal_timing_report(t1, SPACK_NAME" finished in: ", 0); } gnuastro-0.2.33-8a3b/bin/convolve/args.h0000644000175000017500000002000312774160421014624 00000000000000/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef ARGS_H #define ARGS_H #include #include #include "ui.h" /* Definition parameters for the argp: */ const char *argp_program_version=SPACK_STRING"\n"GAL_STRINGS_COPYRIGHT "\n\nWritten by Mohammad Akhlaghi"; const char *argp_program_bug_address=PACKAGE_BUGREPORT; static char args_doc[] = "InputFile"; const char doc[] = /* Before the list of options: */ GAL_STRINGS_TOP_HELP_INFO SPACK_NAME" will convolve an input image with a given spatial kernel " "(image) in the spatial domain (no edge effects) or frequency domain. " "The latter suffers from edge effects, but can be much faster.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /* Free letters for options: c d e g i j l n r t u w x y z A B C E F G H I J O Q R T W X Y Z Free numbers: >=504 */ static struct argp_option options[] = { { 0, 0, 0, 0, "Input:", 1 }, { "mask", 'M', "STR", 0, "Mask image file name.", 1 }, { "mhdu", 'H', "STR", 0, "Mask image header name.", 1 }, { "kernel", 'k', "STR", 0, "Name of kernel for convolution.", 1 }, { "khdu", 'U', "STR", 0, "HDU of kernel file.", 1 }, { "nokernelflip", 500, 0, 0, "Do not flip the kernel image.", 1 }, { "nokernelnorm", 501, 0, 0, "Do not normalize the kernel image.", 1 }, { 0, 0, 0, 0, "Output:", 2 }, { "viewfreqsteps", 'v', 0, 0, "View the steps in the frequency domain.", 2 }, { 0, 0, 0, 0, "Mesh grid (only for spatial domain):", 3 }, { "meshsize", 's', "INT", 0, "Size of each mesh (tile) in the grid.", 3 }, { "nch1", 'a', "INT", 0, "Number of channels along first FITS axis.", 3 }, { "nch2", 'b', "INT", 0, "Number of channels along second FITS axis.", 3 }, { "lastmeshfrac", 'L', "INT", 0, "Fraction of last mesh area to add new.", 3 }, { "checkmesh", 503, 0, 0, "Store mesh IDs in `_mesh.fits' file.", 3 }, { "fullconvolution", 502, 0, 0, "Ignore channels in imageconvolution.", 3 }, { 0, 0, 0, 0, "Operating modes:", -1 }, { "spatial", 'p', 0, 0, "Spatial domain convolution.", -1 }, { "frequency", 'f', 0, 0, "Frequency domain convolution.", -1 }, { "makekernel", 'm', "INT", 0, "Make 2*INT kernel to create input image.", -1 }, {0} }; /* Parse a single option: */ static error_t parse_opt(int key, char *arg, struct argp_state *state) { /* Save the arguments structure: */ struct convolveparams *p = state->input; /* Set the pointer to the common parameters for all programs here: */ state->child_inputs[0]=&p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); switch(key) { /* Inputs: */ case 'M': gal_checkset_allocate_copy_set(arg, &p->up.maskname, &p->up.masknameset); break; case 'H': gal_checkset_allocate_copy_set(arg, &p->up.mhdu, &p->up.mhduset); break; case 'k': gal_checkset_allocate_copy_set(arg, &p->up.kernelname, &p->up.kernelnameset); break; case 'U': gal_checkset_allocate_copy_set(arg, &p->up.khdu, &p->up.khduset); break; case 500: p->kernelflip=0; break; case 501: p->kernelnorm=0; break; /* Output: */ /* Mesh grid: */ case 's': gal_checkset_sizet_l_zero(arg, &p->mp.meshsize, "meshsize", key, SPACK, NULL, 0); p->up.meshsizeset=1; break; case 'a': gal_checkset_sizet_l_zero(arg, &p->mp.nch1, "nch1", key, SPACK, NULL, 0); p->up.nch1set=1; break; case 'b': gal_checkset_sizet_l_zero(arg, &p->mp.nch2, "nch2", key, SPACK, NULL, 0); p->up.nch2set=1; break; case 'L': gal_checkset_float_l_0_s_1(arg, &p->mp.lastmeshfrac, "lastmeshfrac", key, SPACK, NULL, 0); p->up.lastmeshfracset=1; break; case 503: p->meshname="a"; break; case 502: p->mp.fullconvolution=1; p->up.fullconvolutionset=1; break; /* Operating mode: */ case 'p': if(p->up.frequencyset) argp_error(state, "only one of spatial or frequency domain " "convolution modes may be chosen"); p->spatial=1; p->frequency=0; p->up.spatialset=p->up.frequencyset=1; break; case 'f': if(p->up.spatialset) argp_error(state, "only one of spatial or frequency domain " "convolution modes may be chosen"); p->spatial=0; p->frequency=1; p->up.spatialset=p->up.frequencyset=1; break; case 'v': p->viewfreqsteps=1; break; case 'm': gal_checkset_int_el_zero(arg, &p->makekernel, "makekernel", key, SPACK, NULL, 0); p->up.makekernelset=1; break; /* Read the non-option arguments: */ case ARGP_KEY_ARG: if(p->up.inputname) argp_error(state, "only one input file (argument) is required"); p->up.inputname=arg; break; /* The command line options and arguments are finished. */ case ARGP_KEY_END: if(p->cp.setdirconf==0 && p->cp.setusrconf==0 && p->cp.printparams==0) { if(state->arg_num==0) argp_error(state, "no argument given"); if(p->up.inputname==NULL) argp_error(state, "no input files provided"); } break; default: return ARGP_ERR_UNKNOWN; } return 0; } /* Specify the children parsers: */ struct argp_child children[]= { {&commonargp, 0, NULL, 0}, {0, 0, 0, 0} }; /* Basic structure defining the whole argument reading process. */ static struct argp thisargp = {options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif gnuastro-0.2.33-8a3b/bin/convolve/main.h0000644000175000017500000001037212774156226014634 00000000000000/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include #include #include /* Progarm name macros: */ #define SPACK "astconvolve" /* Subpackage executable name. */ #define SPACK_NAME "Convolve" /* Subpackage full name. */ #define SPACK_STRING SPACK_NAME" ("PACKAGE_NAME") "PACKAGE_VERSION #define MINGOODDIVSPEC 0.005 #define CONVFLOATINGPOINTERR 1e-10 #define COMPLEXTOREALSPEC 1 /* Spectrum of complex number. */ #define COMPLEXTOREALPHASE 2 /* Phase of the complex number. */ #define COMPLEXTOREALREAL 3 /* Only show the real part. */ /* User interface parameters structure */ struct uiparams { char *inputname; /* Name of input file. */ char *maskname; /* Mask file name. */ char *mhdu; /* HDU of mask image. */ char *kernelname; /* Name of kernel file. */ char *khdu; /* HDU of input Kernel. */ char *freqstepsname; /* Name of frequency steps file. */ int spatialset; int frequencyset; int masknameset; int mhduset; int kernelnameset; int khduset; int meshsizeset; int nch1set; int nch2set; int lastmeshfracset; int fullconvolutionset; int makekernelset; }; /* Processing parameters structure */ struct convolveparams { struct uiparams up; /* user interface structure. */ struct gal_commonparams cp; /* gal_commonparams structure. */ struct gal_mesh_params mp; /* gal_mesh_params structure. */ /* Inputs: */ int makekernel; /* ==1: Make a kernel to create input. */ float *input; /* Input image array. */ float *kernel; /* Input Kernel array. */ int anyblank; /* If there are blank pixels in input. */ size_t is0; /* Input image size along C's first axis. */ size_t is1; /* Input image size along C's second axis. */ size_t ks0; /* Kernel size along C's first axis. */ size_t ks1; /* Kernel size along C's second axis. */ int kernelflip; /* ==1: Flip the kernel. */ int kernelnorm; /* ==1: Normalize the kernel. */ int nwcs; /* Number of WCS headers. */ struct wcsprm *wcs; /* WCS structure. */ /* Outputs: */ char *meshname; /* Name of mesh structure output. */ /* Operating modes: */ int spatial; /* Convolve using spatial domain. */ int frequency; /* Convolve using frequency domain. */ int viewfreqsteps; /* View the frequency domain steps. */ /* internal: */ time_t rawtime; /* Starting time of the program. */ double *pimg; /* Padded image array. */ double *pker; /* Padded kernel array. */ size_t ps0; /* Padded size along first C axis. */ size_t ps1; /* Padded size along second C axis. */ }; #endif gnuastro-0.2.33-8a3b/bin/convolve/main.c0000644000175000017500000000315312774155617014631 00000000000000/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include /* Includes time.h and sys/time.h */ #include "main.h" #include "convolve.h" #include "ui.h" /* Needs convolveparams in main.h */ int main(int argc, char *argv[]) { struct timeval t1; struct convolveparams p={{0}, {0}, {0}, 0}; /* Set the starting time.*/ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ setparams(argc, argv, &p); /* Run Image Crop */ convolve(&p); /* Free all non-freed allocations. */ freeandreport(&p, &t1); /* Return successfully. */ return EXIT_SUCCESS; } gnuastro-0.2.33-8a3b/bin/convolve/Makefile.in0000644000175000017500000017255513004464626015611 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # 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@GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ REPLACE_READ = @REPLACE_READ@ REPLACE_READLINK = @REPLACE_READLINK@ REPLACE_READLINKAT = @REPLACE_READLINKAT@ REPLACE_REALLOC = @REPLACE_REALLOC@ REPLACE_REALPATH = @REPLACE_REALPATH@ REPLACE_REMAINDER = @REPLACE_REMAINDER@ REPLACE_REMAINDERF = @REPLACE_REMAINDERF@ REPLACE_REMAINDERL = @REPLACE_REMAINDERL@ REPLACE_REMOVE = @REPLACE_REMOVE@ REPLACE_RENAME = @REPLACE_RENAME@ REPLACE_RENAMEAT = @REPLACE_RENAMEAT@ REPLACE_RMDIR = @REPLACE_RMDIR@ REPLACE_ROUND = @REPLACE_ROUND@ REPLACE_ROUNDF = @REPLACE_ROUNDF@ REPLACE_ROUNDL = @REPLACE_ROUNDL@ REPLACE_SETENV = @REPLACE_SETENV@ REPLACE_SETLOCALE = @REPLACE_SETLOCALE@ REPLACE_SIGNBIT = @REPLACE_SIGNBIT@ REPLACE_SIGNBIT_USING_GCC = @REPLACE_SIGNBIT_USING_GCC@ REPLACE_SLEEP = @REPLACE_SLEEP@ REPLACE_SNPRINTF = @REPLACE_SNPRINTF@ REPLACE_SPRINTF = @REPLACE_SPRINTF@ REPLACE_SQRTL = @REPLACE_SQRTL@ REPLACE_STAT = @REPLACE_STAT@ REPLACE_STDIO_READ_FUNCS = @REPLACE_STDIO_READ_FUNCS@ REPLACE_STDIO_WRITE_FUNCS = @REPLACE_STDIO_WRITE_FUNCS@ REPLACE_STPNCPY = @REPLACE_STPNCPY@ REPLACE_STRCASESTR = @REPLACE_STRCASESTR@ REPLACE_STRCHRNUL = @REPLACE_STRCHRNUL@ REPLACE_STRDUP = @REPLACE_STRDUP@ REPLACE_STRERROR = @REPLACE_STRERROR@ REPLACE_STRERROR_R = @REPLACE_STRERROR_R@ REPLACE_STRNCAT = @REPLACE_STRNCAT@ REPLACE_STRNDUP = @REPLACE_STRNDUP@ REPLACE_STRNLEN = @REPLACE_STRNLEN@ REPLACE_STRSIGNAL = @REPLACE_STRSIGNAL@ REPLACE_STRSTR = @REPLACE_STRSTR@ REPLACE_STRTOD = @REPLACE_STRTOD@ REPLACE_STRTOIMAX = @REPLACE_STRTOIMAX@ REPLACE_STRTOK_R = @REPLACE_STRTOK_R@ REPLACE_STRTOUMAX = @REPLACE_STRTOUMAX@ REPLACE_STRUCT_LCONV = @REPLACE_STRUCT_LCONV@ REPLACE_STRUCT_TIMEVAL = @REPLACE_STRUCT_TIMEVAL@ REPLACE_SYMLINK = @REPLACE_SYMLINK@ REPLACE_SYMLINKAT = @REPLACE_SYMLINKAT@ REPLACE_TIMEGM = @REPLACE_TIMEGM@ REPLACE_TMPFILE = @REPLACE_TMPFILE@ REPLACE_TOWLOWER = @REPLACE_TOWLOWER@ REPLACE_TRUNC = @REPLACE_TRUNC@ REPLACE_TRUNCF = @REPLACE_TRUNCF@ REPLACE_TRUNCL = @REPLACE_TRUNCL@ REPLACE_TTYNAME_R = @REPLACE_TTYNAME_R@ REPLACE_UNLINK = @REPLACE_UNLINK@ REPLACE_UNLINKAT = @REPLACE_UNLINKAT@ REPLACE_UNSETENV = @REPLACE_UNSETENV@ REPLACE_USLEEP = @REPLACE_USLEEP@ REPLACE_UTIMENSAT = @REPLACE_UTIMENSAT@ REPLACE_VASPRINTF = @REPLACE_VASPRINTF@ REPLACE_VDPRINTF = @REPLACE_VDPRINTF@ REPLACE_VFPRINTF = @REPLACE_VFPRINTF@ REPLACE_VPRINTF = @REPLACE_VPRINTF@ REPLACE_VSNPRINTF = @REPLACE_VSNPRINTF@ REPLACE_VSPRINTF = @REPLACE_VSPRINTF@ REPLACE_WCRTOMB = @REPLACE_WCRTOMB@ REPLACE_WCSNRTOMBS = @REPLACE_WCSNRTOMBS@ REPLACE_WCSRTOMBS = @REPLACE_WCSRTOMBS@ REPLACE_WCSWIDTH = @REPLACE_WCSWIDTH@ REPLACE_WCTOB = @REPLACE_WCTOB@ REPLACE_WCTOMB = @REPLACE_WCTOMB@ REPLACE_WCWIDTH = @REPLACE_WCWIDTH@ REPLACE_WRITE = @REPLACE_WRITE@ SED = @SED@ SET_MAKE = @SET_MAKE@ SHELL = @SHELL@ SIG_ATOMIC_T_SUFFIX = @SIG_ATOMIC_T_SUFFIX@ SIZE_T_SUFFIX = @SIZE_T_SUFFIX@ STDALIGN_H = @STDALIGN_H@ STDBOOL_H = @STDBOOL_H@ STDDEF_H = @STDDEF_H@ STDINT_H = @STDINT_H@ STRIP = @STRIP@ SYSEXITS_H = @SYSEXITS_H@ SYS_TIME_H_DEFINES_STRUCT_TIMESPEC = @SYS_TIME_H_DEFINES_STRUCT_TIMESPEC@ TIME_H_DEFINES_STRUCT_TIMESPEC = @TIME_H_DEFINES_STRUCT_TIMESPEC@ UINT32_MAX_LT_UINTMAX_MAX = @UINT32_MAX_LT_UINTMAX_MAX@ UINT64_MAX_EQ_ULONG_MAX = @UINT64_MAX_EQ_ULONG_MAX@ UNDEFINE_STRTOK_R = @UNDEFINE_STRTOK_R@ UNISTD_H_DEFINES_STRUCT_TIMESPEC = @UNISTD_H_DEFINES_STRUCT_TIMESPEC@ UNISTD_H_HAVE_WINSOCK2_H = @UNISTD_H_HAVE_WINSOCK2_H@ UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS = @UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS@ VERSION = @VERSION@ WCHAR_T_SUFFIX = @WCHAR_T_SUFFIX@ WINDOWS_64_BIT_OFF_T = @WINDOWS_64_BIT_OFF_T@ WINDOWS_64_BIT_ST_SIZE = @WINDOWS_64_BIT_ST_SIZE@ WINT_T_SUFFIX = @WINT_T_SUFFIX@ YIELD_LIB = @YIELD_LIB@ abs_builddir = @abs_builddir@ abs_srcdir = @abs_srcdir@ abs_top_builddir = @abs_top_builddir@ abs_top_srcdir = @abs_top_srcdir@ ac_ct_AR = @ac_ct_AR@ ac_ct_CC = @ac_ct_CC@ ac_ct_CXX = @ac_ct_CXX@ ac_ct_DUMPBIN = @ac_ct_DUMPBIN@ am__include = @am__include@ am__leading_dot = @am__leading_dot@ am__quote = @am__quote@ am__tar = 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limit (for SysV at least) may be exceeded. .NOEXPORT: gnuastro-0.2.33-8a3b/bin/convolve/astconvolve.conf0000644000175000017500000000176312601570666016752 00000000000000# Default parameters (System) for Convolve. # MakeProfiles is part of GNU Astronomy Utitlies. # # Use the long option name of each paramter followed by # a value. The name and value should be separated by # atleast one of the following charaacters: # space, `,`, `=` or `:` # # Run with `--help` option or read the manual for a full # explanation of what each option means. # # NOTE I: All counting is from zero, not one. # NOTE II: Lines starting with `#` are ignored. # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Operating mode: spatial 0 frequency 1 makekernel 0 # Input: hdu 0 kernel kernel.fits khdu 0 # Output: # Mesh grid: meshsize 32 nch1 1 nch2 1 lastmeshfrac 0.6 fullconvolution 0gnuastro-0.2.33-8a3b/bin/convolve/Makefile.am0000644000175000017500000000271112765246733015574 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. NOTE: $(top_srcdir)/bootstrapped/lib is only necessary ## for internally compiled utilities and libraries. It must not be included ## during the tests since the bootstrapped libraries are not installed. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Utility and its sources bin_PROGRAMS = astconvolve astconvolve_SOURCES = main.c main.h args.h ui.c ui.h convolve.c \ convolve.h cite.h astconvolve_LDADD = $(top_builddir)/bootstrapped/lib/libgnu.la \ -lgnuastro ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astconvolve.conf gnuastro-0.2.33-8a3b/bin/convertt/0000755000175000017500000000000013004464724013615 500000000000000gnuastro-0.2.33-8a3b/bin/convertt/convertt.h0000644000175000017500000000207712616616510015560 00000000000000/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CONVERTT_H #define CONVERTT_H void convertt(struct converttparams *p); #endif gnuastro-0.2.33-8a3b/bin/convertt/convertt.c0000644000175000017500000002374713001632537015556 00000000000000/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include "main.h" #include "jpeg.h" #include "eps.h" /**************************************************************/ /************** Modifying pixel values ***************/ /**************************************************************/ void changevalue(struct converttparams *p) { struct change *tmp, *ttmp; size_t numchange=0, i, j, size; double *from, *to, **ch=p->ch, *d, *df, f, t; /* In case there is no value to convert. */ if(p->change==NULL) return; /* Count the number of conversions, allocate the arrays for them and put the conversion values in it. */ for(tmp=p->change;tmp!=NULL;tmp=tmp->next) ++numchange; errno=0; to=malloc(numchange*sizeof *to); from=malloc(numchange*sizeof *from); if(to==NULL || from==NULL) error(EXIT_FAILURE, errno, "%zu bytes for `to` or `from` in convert", numchange*sizeof *from); i=1; tmp=p->change; while(tmp!=NULL) { to[numchange-i]=tmp->to; from[numchange-i]=tmp->from; ttmp=tmp->next; free(tmp); tmp=ttmp; ++i; } /* Convert the pixel values in the given order: */ size=p->s0[0]*p->s1[0]; for(i=0;inumch;++i) { if(p->isblank[i]) continue; for(j=0;jch; double fluxlow=p->fluxlow, fluxhigh=p->fluxhigh; /* If the flux truncation values are equal, there is no truncation.*/ if(fluxlow==fluxhigh) return; size=p->s0[0]*p->s1[0]; for(i=0;inumch;++i) { if(p->isblank[i]) continue; df=(d=ch[i])+size; do { if(*dfluxhigh) *d=fluxhigh; } while(++dch; double min, max, toadd, *d, *df; size=p->s0[0]*p->s1[0]; for(i=0;inumch;++i) { gal_statistics_d_min_max(ch[i], size, &min, &max); if(p->isblank[i]) continue; if(min<=0.0f) { toadd=-1.0*min+(max-min)/10000.0f; df=(d=ch[i])+size; do *d+=toadd; while(++dnames[0], p->s0[0], p->s1[0], ctime(&p->rawtime), SPACK_STRING); if(p->bitpixs[0]==BYTE_IMG || p->bitpixs[0]==SHORT_IMG || p->bitpixs[0]==LONG_IMG || p->bitpixs[0]==LONGLONG_IMG ) gal_txtarray_array_to_txt(p->ch[0], p->s0[0], p->s1[0], comments, int_cols, accu_cols, ispace, iprec, 'f', p->cp.output); else gal_txtarray_array_to_txt(p->ch[0], p->s0[0], p->s1[0], comments, int_cols, accu_cols, fspace, fprec, 'g', p->cp.output); } void savefits(struct converttparams *p) { void *array; size_t i, size; char hdu[1000]; size=p->s0[0]*p->s1[0]; for(i=0;inumch;++i) { /* Make sure array is in the correct format. */ if(p->bitpixs[i]!=DOUBLE_IMG) gal_fits_change_type(p->ch[i], DOUBLE_IMG, size, p->numnul[i], &array, p->bitpixs[i]); else array=p->ch[i]; /* Write array to a FITS file.*/ sprintf(hdu, "Channel%zu", i+1); gal_fits_array_to_file(p->cp.output, hdu, p->bitpixs[i], array, p->s0[i], p->s1[i], 0, NULL, NULL, SPACK_STRING); /* If array was allocated separately, free it. */ if(p->bitpixs[i]!=DOUBLE_IMG) free(array); } } /**************************************************************/ /************** convert to 8 bit ***************/ /**************************************************************/ void doubleto8bit(struct converttparams *p) { size_t i, size, numch=p->numch; uint8_t *u, *fu, **ech=p->ech, maxbyte=p->maxbyte; double *d, m, tmin, tmax, min=FLT_MAX, max=-FLT_MAX; /* Allocate space for all the channels. */ size=p->s0[0]*p->s1[0]; for(i=0;ich[i], size, &tmin, &tmax); if(i) { if(tminmax) max=tmax; continue; } min=tmin; max=tmax; } /* Change the minimum and maximum if desired, Note that this is only non-redundant when fluxhigh and fluxlow are more or less than the maximum and minimum values in the image.*/ if(p->fluxlow!=p->fluxhigh) { if(p->flminbyte) min=p->fluxlow; if(p->fhmaxbyte) max=p->fluxhigh; } m=(double)maxbyte/(max-min); /* Write the values in the array: */ for(i=0;iisblank[i]) { if(numch==3) /* RGB */ {fu=(u=ech[i])+size; do *u=0; while(++uch[i]; fu=(u=ech[i])+size; if(p->invert) { do { *u = isnan(*d) ? maxbyte : maxbyte-(*d-min)*m; ++d; } while(++uech[i][j]); printf("\b.\n"); } } */ } /**************************************************************/ /************** Main function ***************/ /**************************************************************/ void convertt(struct converttparams *p) { size_t i; /* Make any of the desired changes to the data. */ if(p->changeaftertrunc) { truncateflux(p); changevalue(p); } else { changevalue(p); truncateflux(p); } if(p->log) takelog(p); /* Save the outputs: */ switch(p->outputtype) { case TXTFORMAT: savetxt(p); break; case FITSFORMAT: savefits(p); break; case JPEGFORMAT: doubleto8bit(p); #ifdef HAVE_LIBJPEG savejpeg(p); #else error(EXIT_FAILURE, 0, "you have asked for a JPEG output, however, " "when %s was configured libjpeg was not available. To write " "to JPEG files, libjpeg is required. Please install it and " "configure, make and install %s again", PACKAGE_STRING, PACKAGE_STRING); #endif break; case EPSFORMAT: case PDFFORMAT: doubleto8bit(p); saveepsorpdf(p); break; default: error(EXIT_FAILURE, 0, "a bug! The internal type of the output is " "not recognized. Please contact us so we can find the problem " "and fix it"); } /* Free the ech arrays. Note that if they have not been allocated, they are NULL and free won't complain. */ for(i=0;inumch;++i) free(p->ech[i]); } gnuastro-0.2.33-8a3b/bin/convertt/jpeg.h0000644000175000017500000000226412616616510014637 00000000000000/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef JPEG_H #define JPEG_H int nameisjpeg(char *name); int nameisjpegsuffix(char *name); void preparejpeg(struct converttparams *p, char *filename); void savejpeg(struct converttparams *p); #endif gnuastro-0.2.33-8a3b/bin/convertt/jpeg.c0000644000175000017500000002306013001632537014623 00000000000000/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #ifdef HAVE_LIBJPEG #include #endif #include #include "main.h" #include "jpeg.h" /************************************************************* ************** Acceptable JPEG names ************** *************************************************************/ int nameisjpeg(char *name) { size_t len; len=strlen(name); if ( ( len>=3 && strcmp(&name[len-3], "jpg") == 0 ) || ( len>=3 && strcmp(&name[len-3], "JPG") == 0 ) || ( len>=4 && strcmp(&name[len-4], "jpeg") == 0 ) || ( len>=4 && strcmp(&name[len-4], "JPEG") == 0 ) || ( len>=3 && strcmp(&name[len-3], "jpe") == 0 ) || ( len>=3 && strcmp(&name[len-3], "jif") == 0 ) || ( len>=4 && strcmp(&name[len-4], "jfif") == 0 ) || ( len>=3 && strcmp(&name[len-3], "jfi") == 0 ) ) return 1; else return 0; } int nameisjpegsuffix(char *name) { if (strcmp(name, "jpg") == 0 || strcmp(name, ".jpg") == 0 || strcmp(name, "JPG") == 0 || strcmp(name, ".JPG") == 0 || strcmp(name, "jpeg") == 0 || strcmp(name, ".jpeg") == 0 || strcmp(name, "JPEG") == 0 || strcmp(name, ".JPEG") == 0 || strcmp(name, "jpe") == 0 || strcmp(name, ".jpe") == 0 || strcmp(name, "jif") == 0 || strcmp(name, ".jif") == 0 || strcmp(name, "jfif") == 0 || strcmp(name, ".jfif") == 0 || strcmp(name, "jfi") == 0 || strcmp(name, ".jfi") == 0) return 1; else return 0; } #ifdef HAVE_LIBJPEG /************************************************************* ************** Read a JPEG image ************** *************************************************************/ /* Read the example.c in libjpeg's source code to understand the details of what is going on here. */ struct my_error_mgr { struct jpeg_error_mgr pub; /* "public" fields */ jmp_buf setjmp_buffer; /* for return to caller */ }; typedef struct my_error_mgr *my_error_ptr; METHODDEF(void) jpeg_error_exit(j_common_ptr cinfo) { /* cinfo->err really points to a my_error_mgr struct, so coerce pointer */ my_error_ptr myerr = (my_error_ptr) cinfo->err; /* Always display the message. */ /* We could postpone this until after returning, if we chose. */ (*cinfo->err->output_message) (cinfo); /* Return control to the setjmp point */ longjmp(myerr->setjmp_buffer, 1); } void makejsample(JSAMPLE **a, size_t size) { JSAMPLE *jsarr; if(sizeof *jsarr!=1) { printf("\n\nJSAMPLE has to be unsigned char!\n\n"); exit(EXIT_FAILURE); } errno=0; jsarr=malloc(size*sizeof *jsarr); if(jsarr==NULL) error(EXIT_FAILURE, errno, "%zu bytes for jsarr", size*sizeof *jsarr); *a=jsarr; } double ** readjpg(char *inname, size_t *outs0, size_t *outs1, size_t *numcolors) { double **all; FILE * infile; JSAMPROW jrow; JSAMPLE *jsamp; int rowstride, c; JSAMPARRAY jsarr; struct my_error_mgr jerr; size_t i, j, size, nc, s0, s1; struct jpeg_decompress_struct cinfo; /* Open the input file */ errno=0; if ((infile = fopen(inname, "rb")) == NULL) error(EXIT_FAILURE, errno, "%s", inname); /* Set up the error and decompressing (reading) functions. */ cinfo.err = jpeg_std_error(&jerr.pub); jerr.pub.error_exit = jpeg_error_exit; if (setjmp(jerr.setjmp_buffer)) { jpeg_destroy_decompress(&cinfo); fclose(infile); error(EXIT_FAILURE, 0, "problem in reading %s", inname); } jpeg_create_decompress(&cinfo); jpeg_stdio_src(&cinfo, infile); /* Read the JPEG header information and start de-compressing: */ jpeg_read_header(&cinfo, TRUE); jpeg_start_decompress(&cinfo); /* Get the array width and height and number of color channels: */ s0=*outs0=cinfo.output_height; s1=*outs1=cinfo.output_width; size=s0*s1; nc=*numcolors=cinfo.output_components; rowstride=s1*nc; makejsample(&jsamp, size*nc); /* Allocate all the arrays for each color: */ errno=0; all=malloc(nc*sizeof *all); if(all==NULL) error(EXIT_FAILURE, errno, "%zu bytes for all", nc*sizeof *all); for(i=0;inumch+numcolors>4) error(EXIT_FAILURE, 0, "the number of channels in %s added with the " "previous inputs will exceed 4 (the maximum number of color " "channels). Can't continue", filename); /* Add each channel to the final set of channels. */ for(i=0;is0[p->numch]=s0; p->s1[p->numch]=s1; p->ch[p->numch]=allcolors[i]; p->bitpixs[p->numch]=BYTE_IMG; ++p->numch; } /* Free the array keeping the pointers to each channel. Note that each channel was allocated separately so we can safely remove it.*/ free(allcolors); } /************************************************************* ************** Write a JPEG image ************** *************************************************************/ void writejpeg(JSAMPLE *jsr, struct converttparams *p) { JSAMPROW r[1]; FILE * outfile; int row_stride=0, c; struct jpeg_error_mgr jerr; size_t s0=p->s0[0], s1=p->s1[0]; struct jpeg_compress_struct cinfo; /* Begin the JPEG writing, following libjpeg's example.c */ cinfo.err = jpeg_std_error(&jerr); jpeg_create_compress(&cinfo); errno=0; if ((outfile = fopen(p->cp.output, "wb")) == NULL) error(EXIT_FAILURE, errno, "%s", p->cp.output); jpeg_stdio_dest(&cinfo, outfile); cinfo.image_width = s1; cinfo.image_height = s0; switch(p->numch) { case 1: row_stride=s1; cinfo.input_components = 1; cinfo.in_color_space = JCS_GRAYSCALE; break; case 3: row_stride=3*s1; cinfo.input_components = 3; cinfo.in_color_space = JCS_RGB; break; case 4: row_stride=4*s1; cinfo.input_components = 4; cinfo.in_color_space = JCS_CMYK; break; default: error(EXIT_FAILURE, 0, "a bug! The number of channels in writejpeg " "is not 1, 3 or 4, but %zu. This should not happen. Please " "contact us so we can fix the problem", p->numch); } jpeg_set_defaults(&cinfo); jpeg_set_quality(&cinfo, p->quality, TRUE); cinfo.density_unit=1; cinfo.Y_density=cinfo.X_density=s1/(p->widthincm/2.54); jpeg_start_compress(&cinfo, TRUE); /* cinfo.next_scanline is 'unsigned int' */ c=s0-1; /* In FITS the first row is on the bottom! */ while (cinfo.next_scanline < cinfo.image_height) { r[0] = & jsr[c-- * row_stride]; (void) jpeg_write_scanlines(&cinfo, r, 1); } jpeg_finish_compress(&cinfo); fclose(outfile); jpeg_destroy_compress(&cinfo); } void savejpeg(struct converttparams *p) { JSAMPLE *jsr; uint8_t **ech=p->ech; size_t pixel, color, size, numch=p->numch; /* Make sure the JSAMPLE is 8bits, then allocate the necessary space based on the number of channels. */ if(sizeof *jsr!=1) error(EXIT_FAILURE, 0, "JSAMPLE has to be 8bit"); size=p->numch*p->s0[0]*p->s1[0]; errno=0; jsr=malloc(size*sizeof *jsr); if(jsr==NULL) error(EXIT_FAILURE, errno, "%zu bytes for jsr", size*sizeof *jsr); /* Write the different colors into jsr. */ size=p->s0[0]*p->s1[0]; for(pixel=0;pixel Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef EPS_H #define EPS_H int nameiseps(char *name); int nameisepssuffix(char *name); int nameispdf(char *name); int nameispdfsuffix(char *name); void saveepsorpdf(struct converttparams *p); #endif gnuastro-0.2.33-8a3b/bin/convertt/eps.c0000644000175000017500000002604213001632537014470 00000000000000/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include "main.h" /************************************************************* ************** Acceptable EPS names *************** *************************************************************/ int nameiseps(char *name) { size_t len; len=strlen(name); if ( ( len>=3 && strcmp(&name[len-3], "eps") == 0 ) || ( len>=3 && strcmp(&name[len-3], "EPS") == 0 ) || ( len>=4 && strcmp(&name[len-4], "epsf") == 0 ) || ( len>=4 && strcmp(&name[len-4], "epsi") == 0 ) ) return 1; else return 0; } int nameisepssuffix(char *name) { if (strcmp(name, "eps") == 0 || strcmp(name, ".eps") == 0 || strcmp(name, "EPS") == 0 || strcmp(name, ".EPS") == 0 || strcmp(name, "epsf") == 0 || strcmp(name, ".epsf") == 0 || strcmp(name, "epsi") == 0 || strcmp(name, ".epsi") == 0) return 1; else return 0; } int nameispdf(char *name) { size_t len; len=strlen(name); if (strcmp(&name[len-3], "pdf") == 0 || strcmp(&name[len-3], "PDF") == 0) return 1; else return 0; } int nameispdfsuffix(char *name) { if (strcmp(name, "pdf") == 0 || strcmp(name, ".pdf") == 0 || strcmp(name, "PDF") == 0 || strcmp(name, ".PDF") == 0) return 1; else return 0; } /************************************************************* ************** Write an EPS image ************** *************************************************************/ int onlytwovalues(struct converttparams *p) { uint8_t *i, *fi; fi=(i=p->ech[0])+p->s0[0]*p->s1[0]; do if(*i!=UINT8_MAX && *i!=0) break; while(++i=0;--i) (x&(1<ech[0] into a 0 and 1 bit stream since it only has two values. NOTE: each row has to have an integer number of bytes. */ size_t blackandwhite(struct converttparams *p) { size_t i, j, k; uint8_t *bits, byte, curbit, *ech=p->ech[0]; size_t s0=p->s0[0], s1=p->s1[0], bytesinrow, bytesinimg; /* Find the size values: */ if(p->s1[0]%8) bytesinrow = s1/8 + 1; else bytesinrow = s1/8; bytesinimg=bytesinrow*s0; /* Allocate the array. */ errno=0; bits=calloc(bytesinimg, sizeof *bits); if(bits==NULL) error(EXIT_FAILURE, errno, "allocating %zu bytes in blackandwhite", bytesinimg); for(i=0;i>= 1; } else break; } /*showbits(byte);*/ bits[i*bytesinrow+j]=byte; } } free(p->ech[0]); p->ech[0]=bits; return bytesinimg; } void channelsinhex(struct converttparams *p, FILE *fp, size_t size) { uint8_t *ech; size_t i, j, numelem=35; for(i=0;inumch;++i) { if(p->isblank[i]) fprintf(fp, "{<00>} %% Channel %zu is blank\n", i); else { ech=p->ech[i]; fprintf(fp, "{<"); for(j=0;j}\n"); } } } void channelsinascii85(struct converttparams *p, FILE *fp, size_t size) { uint8_t *ech; uint32_t anint, base; size_t i, j, k, numelem=15; /* 15*5=75 */ for(i=0;inumch;++i) { if(p->isblank[i]) fprintf(fp, "{<00>} %% Channel %zu is blank\n", i); else { ech=p->ech[i]; fprintf(fp, "{<~"); for(j=0;j1) anint+=ech[j+1]*256*256; if(size-j==3) anint+=ech[j+2]*256; } else anint=( ech[j]*256*256*256 + ech[j+1]*256*256 + ech[j+2]*256 + ech[j+3] ); /* If all four bytes are zero, then just print `z'. */ if(anint==0) fprintf(fp, "z"); else { /* To check, just change the fprintf below to printf: printf("\n\n"); printf("%u %u %u %u\n", ech[j], ech[j+1], ech[j+2], ech[j+3]); */ base=85*85*85*85; /* Do the ASCII85 encoding: */ for(k=0;k<5;++k) { fprintf(fp, "%c", anint/base+33); anint%=base; base/=85; } } /* Go to the next line if on the right place: */ if(j%numelem==0) fprintf(fp, "\n"); } fprintf(fp, "~>}\n"); } } } void writeepsimage(struct converttparams *p, FILE *fp) { int bpc=8; size_t i, size; /* Set the number of bits per component. */ if( p->numch==1 && onlytwovalues(p) ) { bpc=1; size=blackandwhite(p); } else size=p->s0[0]*p->s1[0]; if(p->numch==1) fprintf(fp, "/DeviceGray setcolorspace\n"); else if(p->numch==3) fprintf(fp, "/DeviceRGB setcolorspace\n"); else if(p->numch==4) fprintf(fp, "/DeviceCMYK setcolorspace\n"); else error(EXIT_FAILURE, 0, "a bug! In saveepsorpdf the number of channels " "is not 1, 3 or 4. Please contact us so we can find the issue " "and fix it"); fprintf(fp, "<<\n"); fprintf(fp, " /ImageType 1\n"); fprintf(fp, " /Width %zu\n", p->s1[0]); fprintf(fp, " /Height %zu\n", p->s0[0]); fprintf(fp, " /ImageMatrix [ %zu 0 0 %zu 0 0 ]\n", p->s1[0], p->s0[0]); fprintf(fp, " /MultipleDataSources true\n"); fprintf(fp, " /BitsPerComponent %d\n", bpc); fprintf(fp, " /Decode["); for(i=0;inumch;++i) {fprintf(fp, " 0 1");} fprintf(fp, " ]\n"); fprintf(fp, " /Interpolate false\n"); fprintf(fp, " /DataSource [\n"); if(p->hex) channelsinhex(p, fp, size); else channelsinascii85(p, fp, size); fprintf(fp, " ]\n"); fprintf(fp, ">>\n"); fprintf(fp, "image\n\n"); } void saveepsorpdf(struct converttparams *p) { FILE *fp; float hbw; size_t winpt, hinpt; char command[20000], *epsfilename=NULL; /* EPS filename */ if(p->outputtype==EPSFORMAT) { epsfilename=p->cp.output; gal_checkset_check_remove_file(epsfilename, p->cp.dontdelete); } else if (p->outputtype==PDFFORMAT) { gal_checkset_check_remove_file(p->cp.output, p->cp.dontdelete); gal_checkset_automatic_output(p->cp.output, ".ps", 0, p->cp.dontdelete, &epsfilename); } else error(EXIT_FAILURE, 0, "a bug! In `saveeps`, for outputtype is " "neither eps or pdf! Please contact us so we fix it"); /* Find the bounding box */ winpt=p->widthincm*72.0f/2.54f; hinpt=(float)(p->s0[0]*winpt)/(float)(p->s1[0]); hbw=(float)p->borderwidth/2.0f; /* Open the output file and write the top comments. */ errno=0; fp=fopen(epsfilename, "w"); if(fp==NULL) error(EXIT_FAILURE, errno, "%s", p->cp.output); fprintf(fp, "%%!PS-Adobe-3.0 EPSF-3.0\n"); fprintf(fp, "%%%%BoundingBox: 0 0 %zu %zu\n", winpt+2*p->borderwidth, hinpt+2*p->borderwidth); fprintf(fp, "%%%%Creator: %s\n", SPACK_STRING); fprintf(fp, "%%%%CreationDate: %s", ctime(&p->rawtime)); fprintf(fp, "%%%%LanuageLevel: 3\n"); fprintf(fp, "%%%%EndComments\n\n"); if(p->outputtype==EPSFORMAT) fprintf(fp, "gsave\n\n"); /* Commands to draw the border: */ if(p->borderwidth) { fprintf(fp, "%% Draw the border:\n"); fprintf(fp, "0 setgray\n"); fprintf(fp, "%d setlinewidth\n", p->borderwidth); fprintf(fp, "%.1f %.1f moveto\n", hbw, hbw); fprintf(fp, "0 %zu rlineto\n", hinpt+p->borderwidth); fprintf(fp, "%zu 0 rlineto\n", winpt+p->borderwidth); fprintf(fp, "0 -%zu rlineto\n", hinpt+p->borderwidth); fprintf(fp, "closepath\n"); fprintf(fp, "stroke\n\n"); } /* Write the image: */ fprintf(fp, "%% Draw the image:\n"); fprintf(fp, "%d %d translate\n", p->borderwidth, p->borderwidth); fprintf(fp, "%zu %zu scale\n", winpt, hinpt); writeepsimage(p, fp); /* Ending of the EPS file: */ if(p->outputtype==EPSFORMAT) fprintf(fp, "grestore\n"); else fprintf(fp, "showpage\n"); fprintf(fp, "%%%%EOF"); fclose(fp); if(p->outputtype==PDFFORMAT) { sprintf(command, "gs -q -o %s -sDEVICE=pdfwrite -dDEVICEWIDTHPOINTS=%zu" " -dDEVICEHEIGHTPOINTS=%zu -dPDFFitPage %s", p->cp.output, winpt+2*p->borderwidth, hinpt+2*p->borderwidth, epsfilename); if(system(command)) error(EXIT_FAILURE, 0, "the command to convert a PostScript file to " "PDF (`%s') was not successful! The PostScript file (%s) is " "left if you want to convert or use it through any other " "means", command, epsfilename); sprintf(command, "rm %s", epsfilename); if(system(command)) error(EXIT_FAILURE, 0, "The PDF output (%s) was created, but the " "PostScript file which was used to make it (%s) could not be" "removed", p->cp.output, epsfilename); free(epsfilename); } } gnuastro-0.2.33-8a3b/bin/convertt/ui.h0000644000175000017500000000225112616616510014323 00000000000000/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef UI_H #define UI_H struct change * makechangestruct(char *arg); void setparams(int argc, char *argv[], struct converttparams *p); void freeandreport(struct converttparams *p); #endif gnuastro-0.2.33-8a3b/bin/convertt/ui.c0000644000175000017500000005233713002706671014326 00000000000000/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include /* From Gnulib. */ #include /* Includes time.h and sys/time.h */ #include #include "main.h" #include "eps.h" #include "args.h" #include "jpeg.h" /* Set the file names of the places where the default parameters are put. */ #define CONFIG_FILE SPACK CONF_POSTFIX #define SYSCONFIG_FILE SYSCONFIG_DIR "/" CONFIG_FILE #define USERCONFIG_FILEEND USERCONFIG_DIR CONFIG_FILE #define CURDIRCONFIG_FILE CURDIRCONFIG_DIR CONFIG_FILE /**************************************************************/ /************** Options and parameters ***************/ /**************************************************************/ void readconfig(char *filename, struct converttparams *p) { int tmp; FILE *fp; size_t lineno=0, len=200; char *line, *name, *value; struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; char key='a'; /* Not used, just a place holder. */ /* When the file doesn't exist or can't be opened, it is ignored. It might be intentional, so there is no error. If a parameter is missing, it will be reported after all defaults are read. */ fp=fopen(filename, "r"); if (fp==NULL) return; /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); /* Read the tokens in the file: */ while(getline(&line, &len, fp) != -1) { /* Prepare the "name" and "value" strings, also set lineno. */ GAL_CONFIGFILES_START_READING_LINE; /* Inputs: */ if(strcmp(name, "hdu")==0) gal_checkset_allocate_copy_set(value, &cp->hdu, &cp->hduset); else if(strcmp(name, "hdu2")==0) gal_checkset_allocate_copy_set(value, &up->hdu2, &up->hdu2set); else if(strcmp(name, "hdu3")==0) gal_checkset_allocate_copy_set(value, &up->hdu3, &up->hdu3set); else if(strcmp(name, "hdu4")==0) gal_checkset_allocate_copy_set(value, &up->hdu4, &up->hdu4set); /* Outputs: */ else if(strcmp(name, "output")==0) gal_checkset_allocate_copy_set(value, &cp->output, &cp->outputset); else if(strcmp(name, "quality")==0) { if(up->qualityset) continue; gal_checkset_int_smaller_equal_to(value, &p->quality, name, key, p->cp.spack, filename, lineno, 100); if(p->quality<0) error(EXIT_FAILURE, 0, "the quality option should be positive"); up->qualityset=1; } else if(strcmp(name, "widthincm")==0) { if(up->widthincmset) continue; gal_checkset_float_l_0(value, &p->widthincm, name, key, SPACK, filename, lineno); up->widthincmset=1; } else if(strcmp(name, "borderwidth")==0) { if(up->borderwidthset) continue; gal_checkset_int_el_zero(value, &p->borderwidth, name, key, SPACK, filename, lineno); up->borderwidthset=1; } /* Flux: */ else if(strcmp(name, "fluxlow")==0) { if(up->fluxlowset) continue; gal_checkset_any_double(value, &p->fluxlow, name, key, p->cp.spack, filename, lineno); up->fluxlowset=1; } else if(strcmp(name, "fluxhigh")==0) { if(up->fluxhighset) continue; gal_checkset_any_double(value, &p->fluxhigh, name, key, p->cp.spack, filename, lineno); up->fluxhighset=1; } else if(strcmp(name, "maxbyte")==0) { if(up->maxbyteset) continue; gal_checkset_int_smaller_equal_to(value, &tmp, "maxbyte", key, p->cp.spack, NULL, 0, UINT8_MAX); if(tmp<0) error(EXIT_FAILURE, 0, "--maxbyte (-m) should be positive"); p->maxbyte=tmp; p->up.maxbyteset=1; } /* Operating modes: */ /* Read options common to all programs */ GAL_CONFIGFILES_READ_COMMONOPTIONS_FROM_CONF else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s` not recognized.\n", name); } free(line); fclose(fp); } void printvalues(FILE *fp, struct converttparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; /* Print all the options that are set. Separate each group with a commented line explaining the options in that group. */ fprintf(fp, "\n# Input image:\n"); if(cp->hduset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("hdu", cp->hdu); if(up->hdu2set) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("hdu2", up->hdu2); if(up->hdu3set) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("hdu3", up->hdu3); if(up->hdu4set) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("hdu4", up->hdu4); fprintf(fp, "\n# Output parameters:\n"); if(cp->outputset) fprintf(fp, CONF_SHOWFMT"%s\n", "output", cp->output); if(up->qualityset) fprintf(fp, CONF_SHOWFMT"%d\n", "quality", p->quality); if(up->widthincmset) fprintf(fp, CONF_SHOWFMT"%.2f\n", "widthincm", p->widthincm); if(up->borderwidthset) fprintf(fp, CONF_SHOWFMT"%d\n", "borderwidth", p->borderwidth); fprintf(fp, "\n# Output flux display:\n"); if(up->fluxlowset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "fluxlow", p->fluxlow); if(up->fluxhighset) fprintf(fp, CONF_SHOWFMT"%.3f\n", "fluxhigh", p->fluxhigh); if(up->maxbyteset) fprintf(fp, CONF_SHOWFMT"%d\n", "maxbyte", (int)(p->maxbyte)); /* For the operating mode, first put the macro to print the common options, then the (possible options particular to this program). */ fprintf(fp, "\n# Operating modes:\n"); GAL_CONFIGFILES_PRINT_COMMONOPTIONS; } /* Note that numthreads will be used automatically based on the configure time. */ void checkifset(struct converttparams *p) { struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; int intro=0; if(cp->hduset==0) GAL_CONFIGFILES_REPORT_NOTSET("hdu"); if(up->hdu2set==0) GAL_CONFIGFILES_REPORT_NOTSET("hdu2"); if(up->hdu3set==0) GAL_CONFIGFILES_REPORT_NOTSET("hdu3"); if(up->hdu4set==0) GAL_CONFIGFILES_REPORT_NOTSET("hdu4"); if(up->qualityset==0) GAL_CONFIGFILES_REPORT_NOTSET("quality"); if(up->widthincmset==0) GAL_CONFIGFILES_REPORT_NOTSET("widthincm"); if(up->borderwidthset==0) GAL_CONFIGFILES_REPORT_NOTSET("borderwidth"); if(up->fluxlowset==0) GAL_CONFIGFILES_REPORT_NOTSET("fluxlow"); if(up->fluxhighset==0) GAL_CONFIGFILES_REPORT_NOTSET("fluxhigh"); if(up->maxbyteset==0) GAL_CONFIGFILES_REPORT_NOTSET("maxbyte"); GAL_CONFIGFILES_END_OF_NOTSET_REPORT; } /**************************************************************** ***************** Read convert values: ******************** ****************************************************************/ struct change * makechangestruct(char *arg) { char *p=arg; struct change *out=NULL, *c; while(*p!='\0') { while(*p==' ') {++p; continue;} /* Skip all space characters. */ errno=0; c=malloc(sizeof *c); if(c==NULL) error(EXIT_FAILURE, 0, "%zu bytes for struct change", sizeof *c); c->from=strtof(p, &p); while(*p==' ') {++p; continue;} if(*p==':') ++p; else { fprintf(stderr, PACKAGE": In the conversion option, [from] " "and [to] values should be separated by a ':'. You " "have given a '%c': %s\n", *p, arg); exit(EXIT_FAILURE); } c->to=strtof(p, &p); while(*p==' ') {++p; continue;} if(*p==',') p++; else if(*p!='\0') { fprintf(stderr, PACKAGE": In the conversion option, [from] " "and [to] pairs should be separated by a ','. You have " "provided a '%c': %s\n", *p, arg); exit(EXIT_FAILURE); } c->next=out; out=c; } /* { struct change *tmp; for(tmp=out;tmp!=NULL;tmp=tmp->next) printf("%f --> %f\n", tmp->from, tmp->to); } */ return out; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ /* We know cp->output is a known suffix, we just don't know if it has a `.` before it or not. If it doesn't one will be added to it an the output name will be set. */ void adddotautomaticoutput(struct converttparams *p) { size_t i; struct gal_commonparams *cp=&p->cp; char *tmp, *basename="output.txt"; /* Find the first file name in the input(s). */ for(i=0;inuminputs;++i) if(strcmp(p->names[i], BLANKCHANNELNAME)) { basename=p->names[i]; break; } /* If the suffix does not start with a `.`, put one there. */ if(cp->output[0]!='.') { errno=0; tmp=malloc(strlen(cp->output)+10*sizeof *tmp); if(tmp==NULL) error(EXIT_FAILURE, errno, "%zu bytes for suffix name", strlen(cp->output)+10*sizeof *tmp); sprintf(tmp, ".%s", cp->output); free(cp->output); cp->output=tmp; } /* Set the automatic output and make sure we have write access. */ gal_checkset_automatic_output(basename, cp->output, cp->removedirinfo, cp->dontdelete, &cp->output); if( gal_checkset_dir_0_file_1(cp->output, cp->dontdelete)==0 ) error(EXIT_FAILURE, 0, "%s is a directory", cp->output); } void sanitycheck(struct converttparams *p) { size_t i, j; struct gal_commonparams *cp=&p->cp; /* The flux range: */ if(p->fluxlow>p->fluxhigh) error(EXIT_FAILURE, 0, "the value of `--fluxlow` (`-L`, %.3f) is " "larger than `--fluxhigh` (`-H`, %.3f)", p->fluxlow, p->fluxhigh); /* Make sure there are 1 (for grayscale), 3 (for RGB) or 4 (for CMYK) color channels. */ if(p->numch!=1 && p->numch!=3 && p->numch!=4) error(EXIT_FAILURE, 0, "the number of input color channels has to be " "1 (for non image data, grayscale or only K channel in CMYK), " "3 (for RGB) and 4 (for CMYK). You have given %zu color channels. " "Note that some file formats (for example JPEG) can contain more " "than one color channel", p->numch); /* Make sure that there is atleast one input file (not only blank) and set the sizes of the blank channels to the first non-blank value. */ for(i=0;inumch;++i) if(p->isblank[i]==0) break; if(i==p->numch) error(EXIT_FAILURE, 0, "all the input(s) are of type blank"); for(j=0;jnumch;++j) if(p->isblank[j]) { p->s0[j]=p->s0[i]; p->s1[j]=p->s1[i]; } /* Check if all the input sources have the same size: */ if(p->numch>1) { for(i=1;inumch;++i) if(p->s0[i]!=p->s0[0] || p->s1[i]!=p->s1[0]) break; if(i!=p->numch) { for(i=0;inumch;++i) fprintf(stderr, "Channel %zu is %zu x %zu pixels.\n", i, p->s1[i], p->s0[i]); error(EXIT_FAILURE, 0, "the input color channels have different " "sizes"); } } /* Allocate space for the blank channels and set them to zero: */ for(i=0;inumch;++i) if(p->isblank[i]) { errno=0; p->ch[i]=calloc(p->s0[0]*p->s1[0], sizeof *p->ch[i]); if(p->ch[i]==NULL) error(EXIT_FAILURE, errno, "allocating %zu bytes for the blank " "channel %zu", p->s0[0]*p->s1[0]*sizeof *p->ch[i], i); } /* The output file name. First find the first non-blank file name: */ if(cp->outputset) { if(gal_fits_name_is_fits(cp->output)) { p->outputtype=FITSFORMAT; if( gal_fits_suffix_is_fits(cp->output) ) adddotautomaticoutput(p); } else if(nameisjpeg(cp->output)) { #ifndef HAVE_LIBJPEG error(EXIT_FAILURE, 0, "you have asked for a JPEG output, " "however, when %s was configured libjpeg was not " "available. To write to JPEG files, libjpeg is required. " "Please install it and configure, make and install %s " "again", PACKAGE_STRING, PACKAGE_STRING); #else p->outputtype=JPEGFORMAT; if( nameisjpegsuffix(cp->output) ) adddotautomaticoutput(p); #endif } else if(nameiseps(cp->output)) { p->outputtype=EPSFORMAT; if( nameisepssuffix(cp->output) ) adddotautomaticoutput(p); } else if(nameispdf(cp->output)) { p->outputtype=PDFFORMAT; if( nameispdfsuffix(cp->output) ) adddotautomaticoutput(p); } else { /* If the length of the name is shorter than 4 characters, it is most probably a mis-spelled extension, warn the user. */ if(strlen(cp->output)<=5) error(EXIT_FAILURE, 0, "your output file name is " "`%s`, based on its length, it might be a mis-spelled " "extension. Your input is converted to a plain text " "format file with That name", cp->output); p->outputtype=TXTFORMAT; /* If output type is not an image, there should only be one color channel: */ if(p->numch>1) error(EXIT_FAILURE, 0, "text output (`--output=%s`) can only be " "completed with one input color channel. You have given " "%zu. Note that some formats (for example JPEG) can have " "more than one color channel in each file. You can first " "convert the file to FITS, then convert the desired " "channel to text by specifying the HDU", cp->output, p->numch); } } else error(EXIT_FAILURE, 0, "no output file name or extension is specified, " "Please run "SPACK" again with the `--output' or `-o' option.\n\n" "The value to this option doesn't have to be a file name, you " "can also only give an extension (in which case your input file" "name will be used for the base name of the output. For example " "running `"SPACK" filename.fits -ojpg') will produce the output " "file `filename.jpg')"); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ void preparearrays(struct converttparams *p) { size_t i; void *array; double *d, *df; struct gal_linkedlist_stll *tmp; char *hdu=NULL, **names=p->names; /* Put the names in the correct order. */ i=p->numinputs-1; for(tmp=p->inputnames; tmp!=NULL; tmp=tmp->next) names[i--]=tmp->v; p->numch=0; for(i=0;inuminputs;++i) { /* Check if p->numch has not exceeded 4. */ if(p->numch>=4) error(EXIT_FAILURE, 0, "the number of input color channels (not " "files) has exceeded 4! Note that one file can contain more " "than one color channel"); /* Make sure this input file exists (if it isn't blank). */ if(strcmp(names[i], "blank")) gal_checkset_check_file(names[i]); /* FITS: */ if( gal_fits_name_is_fits(names[i]) ) { switch(p->numch) /* Get the HDU value for this channel. */ { case 0: hdu=p->cp.hdu; break; case 1: hdu=p->up.hdu2; break; case 2: hdu=p->up.hdu3; break; case 3: hdu=p->up.hdu4; break; default: error(EXIT_FAILURE, 0, "a bug! In parsing the input " "FITS files, it has gone beyond four! Please " "contact us so we can see what caused this " "problem and fix it"); } p->numnul[p->numch]= gal_fits_hdu_to_array(names[i], hdu, &p->bitpixs[p->numch], &array, &p->s0[p->numch], &p->s1[p->numch]); gal_fits_change_type(array, p->bitpixs[p->numch], p->s0[p->numch]*p->s1[p->numch], p->numnul[p->numch], (void **)(&p->ch[p->numch]), DOUBLE_IMG); free(array); ++p->numch; } /* JPEG: */ else if ( nameisjpeg(names[i]) ) { #ifndef HAVE_LIBJPEG error(EXIT_FAILURE, 0, "you are giving a JPEG input, however, " "when %s was configured libjpeg was not available. To read " "from JPEG files, libjpeg is required. Please install it " "and configure, make and install %s again", PACKAGE_STRING, PACKAGE_STRING); #else preparejpeg(p, names[i]); #endif } /* Blank: */ else if(strcmp(names[i], BLANKCHANNELNAME)==0) { p->isblank[p->numch]=1; p->bitpixs[p->numch]=BYTE_IMG; ++p->numch; } /* EPS: */ else if ( nameiseps(names[i]) ) error(EXIT_FAILURE, 0, "EPS files cannot be used as input. Since " "EPS files are not raster graphics, they are only used as " "output"); /* PDF: */ else if ( nameispdf(names[i]) ) error(EXIT_FAILURE, 0, "PDF files cannot be used as input. Since " "PDF files are not raster graphics, they are only used as " "output"); /* Text: */ else { gal_txtarray_txt_to_array(names[i], &p->ch[p->numch], &p->s0[p->numch], &p->s1[p->numch]); df = (d=p->ch[p->numch]) + p->s0[p->numch]*p->s1[p->numch]; do if(isnan(*d++)) break; while(dbitpixs[p->numch]=DOUBLE_IMG; ++p->numch; } } } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void setparams(int argc, char *argv[], struct converttparams *p) { struct gal_commonparams *cp=&p->cp; /* Set the non-zero initial values, the structure was initialized to have a zero value for all elements. */ cp->spack = SPACK; cp->verb = 1; cp->numthreads = num_processors(NPROC_CURRENT); cp->removedirinfo = 1; p->invert = 1; /* Read the arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Add the user default values and save them if asked. */ GAL_CONFIGFILES_CHECK_SET_CONFIG; /* Check if all the required parameters are set. */ checkifset(p); /* Print the values for each parameter. */ if(cp->printparams) GAL_CONFIGFILES_REPORT_PARAMETERS_SET; /* Prepare the arrays: */ preparearrays(p); /* Do a sanity check. */ sanitycheck(p); } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void freeandreport(struct converttparams *p) { size_t i; struct gal_linkedlist_stll *tmp, *ttmp; free(p->cp.hdu); free(p->up.hdu2); free(p->up.hdu3); free(p->up.hdu4); free(p->cp.output); for(i=0;i<4;++i) free(p->ch[i]); /* Free the input file names: */ tmp=p->inputnames; while(tmp!=NULL) { ttmp=tmp->next; free(tmp); tmp=ttmp; } } gnuastro-0.2.33-8a3b/bin/convertt/cite.h0000644000175000017500000000317312750745735014651 00000000000000/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CITE_H #define CITE_H #define CONVERTTBIBTEX "" #define PRINTCITEABORT { \ printf("\nWe hope %s has been useful for your research.\n" \ "Citations are vital for the continued work on %s.\n" \ "Thank you for citing it in your research paper.\n" \ "\nPlease cite as \"%s\":\n\n%s\n\n%s", \ SPACK_NAME, SPACK_NAME, SPACK_STRING, \ GAL_STRINGS_MAIN_BIBTEX, CONVERTTBIBTEX); \ exit(EXIT_SUCCESS); \ } #endif gnuastro-0.2.33-8a3b/bin/convertt/args.h0000644000175000017500000001734412774157051014660 00000000000000/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef ARGS_H #define ARGS_H #include #include #include "ui.h" /* Definition parameters for the argp: */ const char *argp_program_version=SPACK_STRING"\n"GAL_STRINGS_COPYRIGHT "\n\nWritten by Mohammad Akhlaghi"; const char *argp_program_bug_address=PACKAGE_BUGREPORT; static char args_doc[] = "InputFile1 [InputFile2] ... [InputFile4]"; const char doc[] = /* Before the list of options: */ GAL_STRINGS_TOP_HELP_INFO SPACK_NAME" will convert any of the known input formats to any other " "of the known formats. The output file will have the same number of " "pixels.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /* Free letters for options: d e f g j k p r s t v y z A B E F G I J M O Q R T U W X Y Z Free numbers: 503 */ static struct argp_option options[] = { { 0, 0, 0, 0, "Operating modes:", -1 }, { 0, 0, 0, 0, "Input:", 1 }, { "hdu2", 500, "STR", 0, "HDU of second input FITS image.", 1 }, { "hdu3", 501, "STR", 0, "HDU of third input FITS image.", 1 }, { "hdu4", 502, "STR", 0, "HDU of fourth input FITS image.", 1 }, { 0, 0, 0, 0, "Output:", 2 }, { "quality", 'u', "INT", 0, "Quality of output JPEG image (1 to 100).", 2 }, { "widthincm", 'w', "FLT", 0, "Width in units of centimeters.", 2 }, { "borderwidth", 'b', "FLT", 0, "Border width (EPS, PDF) in units of 1/72 inch.", 2 }, { "hex", 'x', 0, 0, "Hexadecimal encoding in EPS. Default: ASCII85.", 2 }, { 0, 0, 0, 0, "Flux:", 3 }, { "fluxlow", 'L', "FLT", 0, "Lower flux truncation value.", 3 }, { "fluxhigh", 'H', "FLT", 0, "Higher flux truncation value.", 3 }, { "maxbyte", 'm', "INT", 0, "Maximum byte value for all color channels.", 3 }, { "flminbyte", 'i', 0, 0, "Set value of fluxlow as the minimum byte value.", 3 }, { "fhmaxbyte", 'a', 0, 0, "Set value of fluxhigh as the maximum byte value.", 3 }, { "change", 'c', "STR", 0, "Change pixel values `from_1:to_1,from_2:to_2`.", 3 }, { "changeaftertrunc", 'C', 0, 0, "First truncate then change pixel values.", 3 }, { "log", 'l', 0, 0, "Save flux in log scale.", 3 }, { "noinvert", 'n', 0, 0, "Don't invert the image.", 3 }, {0} }; /* Parse a single option: */ static error_t parse_opt(int key, char *arg, struct argp_state *state) { int tmp; /* Save the arguments structure: */ struct converttparams *p = state->input; /* Set the pointer to the common parameters for all programs here: */ state->child_inputs[0]=&p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); switch(key) { /* Input: */ case 500: gal_checkset_allocate_copy_set(arg, &p->up.hdu2, &p->up.hdu2set); break; case 501: gal_checkset_allocate_copy_set(arg, &p->up.hdu3, &p->up.hdu3set); break; case 502: gal_checkset_allocate_copy_set(arg, &p->up.hdu4, &p->up.hdu4set); break; /* Output: */ case 'w': gal_checkset_float_l_0(arg, &p->widthincm, "widthincm", key, p->cp.spack, NULL, 0); p->up.widthincmset=1; break; case 'b': gal_checkset_int_el_zero(arg, &p->borderwidth, "borderwidth", key, p->cp.spack, NULL, 0); p->up.borderwidthset=1; break; case 'u': gal_checkset_int_smaller_equal_to(arg, &p->quality, "quality", key, p->cp.spack, NULL, 0, 100); if(p->quality<0) error(EXIT_FAILURE, 0, "the quality option should be positive"); p->up.qualityset=1; break; case 'x': p->hex=1; break; /* Flux: */ case 'L': gal_checkset_any_double(arg, &p->fluxlow, "fluxlow", key, p->cp.spack, NULL, 0); p->up.fluxlowset=1; break; case 'H': gal_checkset_any_double(arg, &p->fluxhigh, "fluxhigh", key, p->cp.spack, NULL, 0); p->up.fluxhighset=1; break; case 'm': gal_checkset_int_smaller_equal_to(arg, &tmp, "maxbyte", key, p->cp.spack, NULL, 0, UINT8_MAX); if(tmp<0) error(EXIT_FAILURE, 0, "--maxbyte (-m) should be positive"); p->maxbyte=tmp; p->up.maxbyteset=1; break; case 'i': p->flminbyte=1; break; case 'a': p->fhmaxbyte=1; break; case 'c': p->change=makechangestruct(arg); break; case 'C': p->changeaftertrunc=1; break; case 'l': p->log=1; break; case 'n': p->invert=0; break; /* Read the non-option arguments: */ case ARGP_KEY_ARG: gal_linkedlist_add_to_stll(&p->inputnames, arg); ++p->numinputs; break; /* The command line options and arguments are finished. */ case ARGP_KEY_END: if(p->cp.setdirconf==0 && p->cp.setusrconf==0 && p->cp.printparams==0) { if(state->arg_num==0) argp_error(state, "no argument given"); if(p->inputnames==NULL) argp_error(state, "no input files provided"); } break; default: return ARGP_ERR_UNKNOWN; } return 0; } /* Specify the children parsers: */ struct argp_child children[]= { {&commonargp, 0, NULL, 0}, {0, 0, 0, 0} }; /* Basic structure defining the whole argument reading process. */ static struct argp thisargp = {options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif gnuastro-0.2.33-8a3b/bin/convertt/main.h0000644000175000017500000001046612774155570014652 00000000000000/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include #include /* Progarm name macros: */ #define SPACK "astconvertt" /* Subpackage executable name. */ #define SPACK_NAME "ConvertType" /* Subpackage full name. */ #define SPACK_STRING SPACK_NAME" ("PACKAGE_NAME") "PACKAGE_VERSION #define BLANKCHANNELNAME "blank" /* Format codes: */ #define TXTFORMAT -1 #define FITSFORMAT 1 #define JPEGFORMAT 2 #define EPSFORMAT 3 #define PDFFORMAT 4 /* This is used in converting certain values in the array. */ struct change { double from; double to; struct change *next; }; struct uiparams { char *hdu2; /* Header for second FITS image. */ char *hdu3; /* Header for third FITS image. */ char *hdu4; /* Header for fourth FITS image. */ int hdu2set; int hdu3set; int hdu4set; int qualityset; int widthincmset; int borderwidthset; int fluxlowset; int fluxhighset; int maxbyteset; }; struct converttparams { /* Before actual program: */ struct uiparams up; /* User interface parameters. */ struct gal_commonparams cp; /* Common parameters. */ /* Input: */ struct gal_linkedlist_stll *inputnames; /* The names of input files. */ size_t numinputs; /* Number of input files. */ int inputtype; /* The type of the input file. */ /* Output: */ int outputtype; /* The type of the output file. */ int quality; /* Quality of JPEG image. */ float widthincm; /* Width in centimeters. */ int borderwidth; /* Width of border in PostScript points. */ int hex; /* Use hexadecimal not ASCII85 encoding. */ /* Flux: */ double fluxlow; /* Lower flux truncation value. */ double fluxhigh; /* Higher flux truncation value. */ uint8_t maxbyte; /* Maximum byte value. */ int flminbyte; /* fluxlow is minimum byte. */ int fhmaxbyte; /* fluxhigh is maximum byte. */ struct change *change; /* The value conversion string. */ int changeaftertrunc; /* First convert, then truncate. */ int log; /* ==1: Save input in log scale. */ int invert; /* ==1: Invert the image. */ /* INTERNAL PARAMETERS: */ time_t rawtime; /* Starting time of the program. */ /* Input channels: */ char *names[4]; /* File names in input order. */ size_t numch; /* Current Channel. */ int isblank[4]; /* ==1: this channel is blank or fill. */ int bitpixs[4]; /* Bitpix values for each channel. */ int numnul[4]; /* Number of NUL in each channel. */ double *ch[4]; /* Data for each channel. */ uint8_t *ech[4]; /* 8-bit color channels. */ size_t s0[4]; /* First C axis size for each channel. */ size_t s1[4]; /* Second C axis size for each channel. */ }; #endif gnuastro-0.2.33-8a3b/bin/convertt/main.c0000644000175000017500000000306412774155451014637 00000000000000/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include /* Includes time.h and sys/time.h */ #include "main.h" #include "ui.h" /* needs main.h. */ #include "convertt.h" int main(int argc, char *argv[]) { struct converttparams p={{0}, {0}, 0}; /* Set the starting time.*/ time(&p.rawtime); /* Read the input parameters.*/ setparams(argc, argv, &p); /* Run Convert. */ convertt(&p); /* Free all non-freed allocations. */ freeandreport(&p); /* Return successfully.*/ return EXIT_SUCCESS; } gnuastro-0.2.33-8a3b/bin/convertt/Makefile.in0000644000175000017500000017305013004464626015611 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # This 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= @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ 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uninstall-am uninstall-binPROGRAMS uninstall-dist_sysconfDATA .PRECIOUS: Makefile # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: gnuastro-0.2.33-8a3b/bin/convertt/astconvertt.conf0000644000175000017500000000177012500255530016756 00000000000000# Default parameters (System) for ConvertType. # MakeProfiles is part of GNU Astronomy Utitlies. # # Use the long option name of each paramter followed by # a value. The name and value should be separated by # atleast one of the following charaacters: # space, `,`, `=` or `:` # # Run with `--help` option or read the manual for a full # explanation of what each option means. # # NOTE I: All counting is from zero, not one. # NOTE II: Lines starting with `#` are ignored. # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Input: hdu 0 hdu2 0 hdu3 0 hdu4 0 # Output: quality 100 widthincm 10.0 borderwidth 1 output jpg # Flux: fluxlow 0.0 fluxhigh 0.0 maxbyte 255 gnuastro-0.2.33-8a3b/bin/convertt/Makefile.am0000644000175000017500000000274012765246630015603 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. NOTE: $(top_srcdir)/bootstrapped/lib is only necessary ## for internally compiled utilities and libraries. It must not be included ## during the tests since the bootstrapped libraries are not installed. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Utility and its sources bin_PROGRAMS = astconvertt astconvertt_SOURCES = main.c main.h args.h cite.h ui.c ui.h eps.c \ eps.h jpeg.c jpeg.h convertt.c convertt.h astconvertt_LDADD = $(top_builddir)/bootstrapped/lib/libgnu.la \ -lgnuastro ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astconvertt.conf gnuastro-0.2.33-8a3b/bin/arithmetic/0000755000175000017500000000000013004464724014102 500000000000000gnuastro-0.2.33-8a3b/bin/arithmetic/arithmetic.h0000644000175000017500000000210312722534072016320 00000000000000/********************************************************************* ImageArithmetic - Do arithmetic operations on images. ImageArithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef IMGARITH_H #define IMGARITH_H void imgarith(struct imgarithparams *p); #endif gnuastro-0.2.33-8a3b/bin/arithmetic/arithmetic.c0000644000175000017500000010265413001632537016323 00000000000000/********************************************************************* ImageArithmetic - Do arithmetic operations on images. ImageArithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include "main.h" #include "arithmetic.h" /* needs main.h. */ /***************************************************************/ /************* Operand linked list functions *************/ /***************************************************************/ size_t num_operands(struct imgarithparams *p) { size_t counter=0; struct operand *tmp=NULL; for(tmp=p->operands;tmp!=NULL;tmp=tmp->next) ++counter; return counter; } void add_operand(struct imgarithparams *p, char *filename, double number, double *array) { struct operand *newnode; /* Allocate space for the new operand. */ errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "imgarith.c: Making new element in operand"); /* Fill in the values. */ newnode->array=array; newnode->number=number; newnode->filename=filename; if(filename != NULL && gal_fits_name_is_fits(filename)) { /* Set the HDU for this filename. */ gal_linkedlist_pop_from_stll(&p->hdus, &newnode->hdu); /* Increment the FITS counter. */ ++p->addcounter; } /* Make the link to the previous list. */ newnode->next=p->operands; p->operands=newnode; } void pop_operand(struct imgarithparams *p, double *number, double **array, char *operator) { int bitpix; size_t s0, s1; struct uiparams *up=&p->up; struct operand *operands=p->operands; char *maskname, *mhdu, *filename, *hdu; /* If the operand linked list has finished, then give an error and exit. */ if(operands==NULL) error(EXIT_FAILURE, 0, "not enough operands for the \"%s\" operator", operator); /* Set the array output. If filename is present then read the file and fill in the array, if not then just set the array. */ if(strlen(operands->filename)) { hdu=operands->hdu; filename=operands->filename; /* In case this is the first image that is read, then read the WCS information and set the mask name so masked pixels can be set to NaN. For the other images, the mask can be completely ignored. */ if(p->popcounter) /* This is not the first FITS file. */ { maskname=NULL; mhdu=NULL; } else { mhdu=up->mhdu; maskname=up->maskname; gal_fits_read_wcs(filename, hdu, 0, 0, &p->nwcs, &p->wcs); } gal_fits_file_to_double(filename, maskname, hdu, mhdu, array, &bitpix, &p->anyblank, &s0, &s1); /* If the output size was not set yet, then set it. Otherwise, make sure the size of this image is the same as the previous images. */ if(p->s0==0 && p->s1==0) { p->s0=s0; p->s1=s1; } else { if(p->s0!=s0 || p->s1!=s1) error(EXIT_FAILURE, 0, "%s (hdu=%s): has size of %zu x %zu. " "However, previous images had a size of %zu x %zu. All " "the images must be the same size in order for " "ImageArithmetic to work", filename, hdu, s0, s1, p->s0, p->s1); } /* Free the HDU string: */ free(hdu); /* Add to the number of popped FITS images: */ ++p->popcounter; /* Report the read image if desired: */ if(p->cp.verb) printf("%s is read.\n", filename); } else *array=operands->array; /* Set the number: */ *number=operands->number; /* Remove this node from the queue. */ p->operands=operands->next; free(operands); } /***************************************************************/ /************* Operators *************/ /***************************************************************/ void sum(struct imgarithparams *p) { size_t size; char *operator="+"; double fnum, snum; /* First or second number. */ double *farr, *sarr; /* First or second array. */ /* Pop out the number of operands needed. */ pop_operand(p, &fnum, &farr, operator); pop_operand(p, &snum, &sarr, operator); /* Set the total number of pixels, note that we can't do this in the definition of the variable because p->s0 and p->s1 will be set in pop_operand for the first image. */ size=p->s0*p->s1; /* Do the operation: */ if(farr && sarr) /* Both are arrays. */ { /* Do the operation, note that the output is stored in the first input. */ gal_array_dsum_arrays(farr, sarr, size); /* Push the output onto the stack. */ add_operand(p, NOOPTFILENAME, NOOPTNUMBER, farr); /* Clean up. */ free(sarr); } else if(farr) /* Only the first is an array. */ { gal_array_dsum_const(farr, size, snum); add_operand(p, NOOPTFILENAME, NOOPTNUMBER, farr); } else if(sarr) /* Only the first is an array. */ { gal_array_dsum_const(sarr, size, fnum); add_operand(p, NOOPTFILENAME, NOOPTNUMBER, sarr); } else /* Both are numbers. */ add_operand(p, NOOPTFILENAME, fnum+snum, NOOPTARRAY); } void subtract(struct imgarithparams *p) { size_t size; char *operator="-"; double fnum, snum; /* First or second number. */ double *farr, *sarr; /* First or second array. */ /* Pop out the number of operands needed. */ pop_operand(p, &fnum, &farr, operator); pop_operand(p, &snum, &sarr, operator); /* Set the total number of pixels, note that we can't do this in the definition of the variable because p->s0 and p->s1 will be set in pop_operand for the first image. */ size=p->s0*p->s1; /* Do the operation: */ if(farr && sarr) /* Both are arrays. */ { /* Do the operation, note that the output is stored in the first input. Also note that since the linked list is first-in-first-out, the second operand should be put first here. */ gal_array_dsubtract_arrays(sarr, farr, size); /* Push the output onto the stack. */ add_operand(p, NOOPTFILENAME, NOOPTNUMBER, sarr); /* Clean up. */ free(farr); } else if(farr) /* Only the first is an array. */ { gal_array_dconst_subtract(farr, size, snum); add_operand(p, NOOPTFILENAME, NOOPTNUMBER, farr); } else if(sarr) /* Only the first is an array. */ { gal_array_dsubtract_const(sarr, size, fnum); add_operand(p, NOOPTFILENAME, NOOPTNUMBER, sarr); } else /* Both are numbers. */ add_operand(p, NOOPTFILENAME, snum-fnum, NOOPTARRAY); } void multiply(struct imgarithparams *p) { size_t size; char *operator="*"; double fnum, snum; /* First or second number. */ double *farr, *sarr; /* First or second array. */ /* Pop out the number of operands needed. */ pop_operand(p, &fnum, &farr, operator); pop_operand(p, &snum, &sarr, operator); /* Set the total number of pixels, note that we can't do this in the definition of the variable because p->s0 and p->s1 will be set in pop_operand for the first image. */ size=p->s0*p->s1; /* Do the operation: */ if(farr && sarr) /* Both are arrays. */ { /* Do the operation, note that the output is stored in farr. */ gal_array_dmultip_arrays(farr, sarr, size); /* Push the output onto the stack. */ add_operand(p, NOOPTFILENAME, NOOPTNUMBER, farr); /* Clean up. */ free(sarr); } else if(farr) /* Only the first is an array. */ { gal_array_dmultip_const(farr, size, snum); add_operand(p, NOOPTFILENAME, NOOPTNUMBER, farr); } else if(sarr) /* Only the first is an array. */ { gal_array_dmultip_const(sarr, size, fnum); add_operand(p, NOOPTFILENAME, NOOPTNUMBER, sarr); } else /* Both are numbers. */ add_operand(p, NOOPTFILENAME, fnum*snum, NOOPTARRAY); } void divide(struct imgarithparams *p) { size_t size; char *operator="/"; double fnum, snum; /* First or second number. */ double *farr, *sarr; /* First or second array. */ /* Pop out the number of operands needed. */ pop_operand(p, &fnum, &farr, operator); pop_operand(p, &snum, &sarr, operator); /* Set the total number of pixels, note that we can't do this in the definition of the variable because p->s0 and p->s1 will be set in pop_operand for the first image. */ size=p->s0*p->s1; /* Do the operation: */ if(farr && sarr) /* Both are arrays. */ { /* Do the operation, note that the output is stored in the first input. Also note that since the linked list is first-in-first-out, the second operand should be put first here. */ gal_array_ddivide_arrays(sarr, farr, size); /* Push the output onto the stack. */ add_operand(p, NOOPTFILENAME, NOOPTNUMBER, sarr); /* Clean up. */ free(farr); } else if(farr) /* Only the first is an array. */ { gal_array_dconst_divide(farr, size, snum); add_operand(p, NOOPTFILENAME, NOOPTNUMBER, farr); } else if(sarr) /* Only the first is an array. */ { gal_array_ddivide_const(sarr, size, fnum); add_operand(p, NOOPTFILENAME, NOOPTNUMBER, sarr); } else /* Both are numbers. */ add_operand(p, NOOPTFILENAME, snum/fnum, NOOPTARRAY); } void topower(struct imgarithparams *p, char *op) { size_t size; char *operator = op?op:"pow"; double fnum, snum; /* First or second number. */ double *farr, *sarr; /* First or second array. */ /* Pop out the number of operands needed. */ pop_operand(p, &fnum, &farr, operator); pop_operand(p, &snum, &sarr, operator); /* Set the total number of pixels, note that we can't do this in the definition of the variable because p->s0 and p->s1 will be set in pop_operand for the first image. */ size=p->s0*p->s1; /* Do the operation: */ if(farr && sarr) /* Both are arrays. */ { /* Do the operation, note that the output is stored in the first input. Also note that since the linked list is first-in-first-out, the second operand should be put first here. */ gal_array_dpower_arrays(sarr, farr, size); /* Push the output onto the stack. */ add_operand(p, NOOPTFILENAME, NOOPTNUMBER, sarr); /* Clean up. */ free(farr); } else if(farr) /* Only the first is an array. */ { gal_array_dconst_power(farr, size, snum); add_operand(p, NOOPTFILENAME, NOOPTNUMBER, farr); } else if(sarr) /* Only the first is an array. */ { gal_array_dpower_const(sarr, size, fnum); add_operand(p, NOOPTFILENAME, NOOPTNUMBER, sarr); } else /* Both are numbers. */ add_operand(p, NOOPTFILENAME, pow(snum, fnum), NOOPTARRAY); } void alloppixs(struct imgarithparams *p, char *operator) { int i, j; /* Integer to allow negative checks. */ double num; /* Temporary number holder. */ double *arr; /* Temporary array holder. */ int firstisarray=-1; /* ==-1: unset. ==1: array. ==0: number. */ double *allpixels=NULL; /* Array for all values in one pixel. */ double **allarrays=NULL; /* Array for pointers to input arrays. */ size_t size, numop=num_operands(p); double (*thisfunction)(double *, size_t)=NULL; /* First set the appropriate function to call. */ if(!strcmp(operator, "min")) thisfunction = &gal_statistics_double_min_return; else if(!strcmp(operator, "max")) thisfunction = &gal_statistics_double_max_return; else if(!strcmp(operator, "median")) thisfunction = &gal_statistics_median_double_in_place; else if(!strcmp(operator, "average")) thisfunction = &gal_statistics_double_average; else error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we " "can address the problem. The value of `operator' in " "alloppixs (%s) is not recognized", PACKAGE_BUGREPORT, operator); /* Allocate the array of pointers to all input arrays and also the array to temporarily keep all values for each pixel */ errno=0; allarrays=malloc(numop*sizeof *allarrays); if(allarrays==NULL) error(EXIT_FAILURE, errno, "%zu bytes for allarrays in alloppixs", numop*sizeof *allarrays); errno=0; allpixels=malloc(numop*sizeof *allpixels); if(allpixels==NULL) error(EXIT_FAILURE, errno, "%zu bytes for allpixels in alloppixs", numop*sizeof *allpixels); /* Prepare all the inputs, note that since it is a linked list, the operands pop from the last to first. Here order is not important, but in other cases that it might be (and also for debugging), here the inputs are put in order so the indexs start from the last to first. */ for(i=numop-1;i>=0;--i) { /* Pop out the operand. */ pop_operand(p, &num, &arr, operator); /* Do the appropriate action if it is an array or a number. */ if(arr) switch(firstisarray) { case -1: firstisarray=1; allarrays[i]=arr; break; case 1: allarrays[i]=arr; break; case 0: error(EXIT_FAILURE, 0, "for the %s operator, all operands " "must be either an array or number", operator); break; default: error(EXIT_FAILURE, 0, "a Bug! Please contact us at %s so we " "can address the problem. The value of firstisarray (%d) " "in the alloppixs function is not recognized", PACKAGE_BUGREPORT, firstisarray); } else switch(firstisarray) { case -1: firstisarray=0; allpixels[i]=num; break; case 0: allpixels[i]=num; break; case 1: error(EXIT_FAILURE, 0, "for the %s operator, all operands " "must be either an array or number", operator); break; default: error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we " "can address the problem. The value of firstisarray (%d) " "in the alloppixs function is not recognized", PACKAGE_BUGREPORT, firstisarray); } } /* Set the total number of pixels, note that we can't do this in the definition of the variable because p->s0 and p->s1 will be set in pop_operand for the first image. */ size=p->s0*p->s1; /* Do the operation and report the result: */ if(arr) { /* Find the value and replace it with the first operand. */ for(i=0;is0*p->s1); /* Push the output onto the stack. */ add_operand(p, NOOPTFILENAME, NOOPTNUMBER, farr); } else /* Operand is a number. */ add_operand(p, NOOPTFILENAME, log(fnum), NOOPTARRAY); } void takelog10(struct imgarithparams *p) { char *operator="log10"; double fnum, *farr; /* Pop out the number of operands needed. */ pop_operand(p, &fnum, &farr, operator); /* Do the operation: */ if(farr) /* Operand is array. */ { /* Do the operation, note that the output is stored in the first input. Also note that since the linked list is first-in-first-out, the second operand should be put first here. */ gal_array_dlog10_array(farr, p->s0*p->s1); /* Push the output onto the stack. */ add_operand(p, NOOPTFILENAME, NOOPTNUMBER, farr); } else /* Operand is a number. */ add_operand(p, NOOPTFILENAME, log10(fnum), NOOPTARRAY); } void takeabs(struct imgarithparams *p) { char *operator="abs"; double fnum, *farr; /* Pop out the number of operands needed. */ pop_operand(p, &fnum, &farr, operator); /* Do the operation: */ if(farr) /* Operand is array. */ { /* Do the operation, note that the output is stored in the first input. Also note that since the linked list is first-in-first-out, the second operand should be put first here. */ gal_array_dabs_array(farr, p->s0*p->s1); /* Push the output onto the stack. */ add_operand(p, NOOPTFILENAME, NOOPTNUMBER, farr); } else /* Operand is a number. */ add_operand(p, NOOPTFILENAME, fabs(fnum), NOOPTARRAY); } void findmin(struct imgarithparams *p) { char *operator="min"; double min, fnum, *farr; /* Pop out the number of operands needed. */ pop_operand(p, &fnum, &farr, operator); /* Do the operation: */ if(farr) /* Operand is array. */ { /* Do the operation, note that the output is stored in the first input. Also note that since the linked list is first-in-first-out, the second operand should be put first here. */ gal_statistics_double_min(farr, p->s0*p->s1, &min); /* Push the output onto the stack. */ add_operand(p, NOOPTFILENAME, min, NOOPTARRAY); /* Clean up. */ free(farr); } else /* Operand is a number. */ add_operand(p, NOOPTFILENAME, fnum, NOOPTARRAY); } void findmax(struct imgarithparams *p) { char *operator="max"; double max, fnum, *farr; /* Pop out the number of operands needed. */ pop_operand(p, &fnum, &farr, operator); /* Do the operation: */ if(farr) /* Operand is array. */ { /* Do the operation, note that the output is stored in the first input. Also note that since the linked list is first-in-first-out, the second operand should be put first here. */ gal_statistics_double_max(farr, p->s0*p->s1, &max); /* Push the output onto the stack. */ add_operand(p, NOOPTFILENAME, max, NOOPTARRAY); /* Clean up. */ free(farr); } else /* Operand is a number. */ add_operand(p, NOOPTFILENAME, fnum, NOOPTARRAY); } int lessthan(double left, double right) { return leftright; } int greaterequal(double left, double right) { return left>=right; } int equal(double left, double right) { return left==right; } int notequal(double left, double right) { return left!=right; } void conditionals(struct imgarithparams *p, char *operator) { size_t size; double fnum, snum; /* First or second number. */ double *farr, *sarr; /* First or second array. */ double *f, *s, *ff, *ss; int (*thisfunction)(double, double)=NULL; /* Pop out the number of operands needed. */ pop_operand(p, &fnum, &farr, operator); pop_operand(p, &snum, &sarr, operator); /* Set the total number of pixels, note that we can't do this in the definition of the variable because p->s0 and p->s1 will be set in pop_operand for the first image. */ size=p->s0*p->s1; if(!strcmp(operator, "lt")) thisfunction = &lessthan; else if(!strcmp(operator, "le")) thisfunction = &lessequal; else if(!strcmp(operator, "gt")) thisfunction = &greaterthan; else if(!strcmp(operator, "ge")) thisfunction = &greaterequal; else if(!strcmp(operator, "eq")) thisfunction = &equal; else if(!strcmp(operator, "neq")) thisfunction = ¬equal; else error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we " "can address the problem. The value of `operator' in " "conditionals (%s) is not recognized", PACKAGE_BUGREPORT, operator); /* Do the operation: */ if(farr && sarr) /* Both are arrays. */ { /* Do the operation, note that the output is stored in the first input. Also note that since the linked list is first-in-first-out, the second operand should be put first here. */ f=farr; ss=(s=sarr)+size; do *s = thisfunction(*s, *f++); while(++ss0*p->s1; if(!strcmp(operator, "and")) do *f = *s++ && *f; while(++fs0*p->s1; do *f = !(*f); while(++fs0 and p->s1 will be set in pop_operand for the first image. */ size=p->s0*p->s1; /* Do the operation: */ if(farr) /* Operand is array. */ { /* Do the operation, note that the output is stored in the first input. Also note that since the linked list is first-in-first-out, the second operand should be put first here. */ ff=(f=farr)+size; do *f = isnan(*f); while(++fs0 and p->s1 will be set in pop_operand for the first image. */ size=p->s0*p->s1; /* Do the operation: */ if(iarr && carr) /* Both are arrays. */ { c=carr; ii=(i=iarr)+size; if(narr) /* `new' is an array, not number. */ { n=narr; /* Note that we need to increment "f" after the check and replace. If the increment is inside the conditional replace, then when t==0, the increment won't work.*/ do {*i = *c++ ? *n : *i; ++n;} while(++is0=p->s1=0; p->operands=NULL; p->addcounter=p->popcounter=0; /* Go over each input token and do the work. */ for(token=p->tokens;token!=NULL;token=token->next) { /* If we have a name or number, then add it to the operands linked list. Otherwise, pull out two members and do the specified operation on them. */ if(gal_fits_name_is_fits(token->v)) add_operand(p, token->v, NOOPTNUMBER, NOOPTARRAY); else if(gal_checkset_str_is_double(token->v, &number)) add_operand(p, NOOPTFILENAME, number, NOOPTARRAY); else { if (!strcmp(token->v, "+")) sum(p); else if(!strcmp(token->v, "-")) subtract(p); else if(!strcmp(token->v, "*")) multiply(p); else if(!strcmp(token->v, "/")) divide(p); else if(!strcmp(token->v, "abs")) takeabs(p); else if(!strcmp(token->v, "pow")) topower(p, NULL); else if(!strcmp(token->v, "sqrt")) takesqrt(p); else if(!strcmp(token->v, "log")) takelog(p); else if(!strcmp(token->v, "log10")) takelog10(p); else if(!strcmp(token->v, "minvalue")) findmin(p); else if(!strcmp(token->v, "maxvalue")) findmax(p); else if(!strcmp(token->v, "min") || !strcmp(token->v, "max") || !strcmp(token->v, "average") || !strcmp(token->v, "median")) alloppixs(p, token->v); else if(!strcmp(token->v, "lt") || !strcmp(token->v, "le") || !strcmp(token->v, "gt") || !strcmp(token->v, "ge") || !strcmp(token->v, "eq") || !strcmp(token->v, "neq")) conditionals(p, token->v); else if(!strcmp(token->v, "and") || !strcmp(token->v, "or")) andor(p, token->v); else if(!strcmp(token->v, "not")) notfunc(p); else if(!strcmp(token->v, "isblank")) opisblank(p); else if(!strcmp(token->v, "where")) where(p); else error(EXIT_FAILURE, 0, "the argument \"%s\" could not be " "interpretted as an operator", token->v); } } /* If there is more than one node in the operands stack, then the user has given too many operands and there is an error. */ if(p->operands->next!=NULL) error(EXIT_FAILURE, 0, "there are too many operands for the operators " "in the given expression"); /* If the remaining operand is an array then save the array as a FITS image, if not, simply print the floating point number. */ if(p->operands->array) { /* Internally, all arrays were double type. But the user could set the the output type using the type option. So if the user has asked for anything other than a double, we will have to convert the arrays.*/ if(p->type==DOUBLE_IMG) gal_fits_array_to_file(p->cp.output, "astimgarith", DOUBLE_IMG, p->operands->array, p->s0, p->s1, p->anyblank, p->wcs, NULL, SPACK_STRING); else { gal_fits_change_type(p->operands->array, DOUBLE_IMG, p->s0*p->s1, p->anyblank, &array, p->type); gal_fits_array_to_file(p->cp.output, "astimgarith", p->type, array, p->s0, p->s1, p->anyblank, p->wcs, NULL, SPACK_STRING); free(array); } free(p->operands->array); } else printf("%g\n", p->operands->number); /* If there are any remaining HDUs in the hdus linked list, then free them. */ while(p->hdus!=NULL) { gal_linkedlist_pop_from_stll(&p->hdus, &tokeepvalue); free(tokeepvalue); } } /***************************************************************/ /************* Top function *************/ /***************************************************************/ void imgarith(struct imgarithparams *p) { reversepolish(p); } gnuastro-0.2.33-8a3b/bin/arithmetic/args.h0000644000175000017500000001507012774157037015143 00000000000000/********************************************************************* ImageArithmetic - Do arithmetic operations on images. ImageArithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef ARGS_H #define ARGS_H #include #include #include #include /**************************************************************/ /************** argp.h definitions ***************/ /**************************************************************/ /* Definition parameters for the argp: */ const char *argp_program_version=SPACK_STRING"\n"GAL_STRINGS_COPYRIGHT "\n\nWritten by Mohammad Akhlaghi"; const char *argp_program_bug_address=PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata or number [ASTRdata] OPERATOR ..."; const char doc[] = /* Before the list of options: */ GAL_STRINGS_TOP_HELP_INFO SPACK_NAME" will do arithmetic operations on one or multiple images and " "numbers. Simply put, the name of the image along with the arithmetic " "operators and possible numbers are given as arguments. The extensions of " "each input image are expected as options (starting with `hdu') listed " "below. Please note that currently "SPACK_NAME" only supports postfix " "or reverse polish notation. For example to get the result of `5+6', you " "should write `5 6 +', or to get the average of two images, you should " "write `a.fits b.fits + 2 /' (or more simply a.fits b.fits average). " "Please see the manual for more information. " "\n\nThe operators/functions recognized by "SPACK_NAME" are: +, -, *, /, " "abs, pow, sqrt, log, log10, minvalue, maxvalue, min, max, average, median, " "lt, le, gt, ge, eq, neq, and, or, not, isblank. Please run `info gnuastro " "\"Arithmetic operators\"' for detailed information on each operator. Note " "that multiplication should be quoted (like \"*\", or '*') to avoid shell " "expansion.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /* Available letters for short options: a b c d e f g i j k l m n p r s t u v w x y z A B C E F G H I J L O Q R U W X Y Z Number keys used: <=500 Options with keys (second structure element) larger than 500 do not have a short version. */ static struct argp_option options[] = { { 0, 0, 0, 0, "Input:", 1 }, { "hdu", 'h', "STR", 0, "Nth call of this option, used for Nth input FITS.", 1 }, { "mask", 'M', "STR", 0, "Mask image file name.", 1 }, { "mhdu", 'H', "STR", 0, "Mask image header name.", 1 }, { 0, 0, 0, 0, "Output:", 2 }, { "type", 'T', "STR", 0, "byte, short, long, longlong, float, double.", 2 }, { 0, 0, 0, 0, "Operating modes:", -1 }, {0} }; /* Parse a single option: */ static error_t parse_opt(int key, char *arg, struct argp_state *state) { /* Save the arguments structure: */ char *tokeephdu; struct imgarithparams *p = state->input; /* Set the pointer to the common parameters for all programs here: */ state->child_inputs[0]=&p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); switch(key) { /* Commandline options don't need to be allocated, since they are already in static memory and their pointers will not change. They also don't need to be freed for the same reason. However, later on, we will also be reading from the configuration files and there, we need to allocate space (and free it later). So to consistently free all the poped strings, we are allocating a copy here too. */ case 'h': gal_checkset_allocate_copy(arg, &tokeephdu); gal_linkedlist_add_to_stll(&p->hdus, tokeephdu); break; /* Input: */ case 'M': gal_checkset_allocate_copy_set(arg, &p->up.maskname, &p->up.masknameset); break; case 'H': gal_checkset_allocate_copy_set(arg, &p->up.mhdu, &p->up.mhduset); break; /* Output */ case 'T': gal_checkset_known_types(arg, &p->type, NULL, 0); p->up.typeset=1; break; /* Operating modes: */ /* Read the non-option arguments: */ case ARGP_KEY_ARG: /* Add the argument to the list of tokens: */ gal_linkedlist_add_to_stll(&p->tokens, arg); break; /* The command line options and arguments are finished. */ case ARGP_KEY_END: if(p->cp.setdirconf==0 && p->cp.setusrconf==0 && p->cp.printparams==0) { if(state->arg_num==0) argp_error(state, "no argument given"); } break; default: return ARGP_ERR_UNKNOWN; } return 0; } /* Specify the children parsers: */ struct argp_child children[]= { {&commonargp, 0, NULL, 0}, {0, 0, 0, 0} }; /* Basic structure defining the whole argument reading process. */ static struct argp thisargp = {options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif gnuastro-0.2.33-8a3b/bin/arithmetic/ui.h0000644000175000017500000000213412722534072014610 00000000000000/********************************************************************* ImageArithmetic - Do arithmetic operations on images. ImageArithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef IMCROPUI_H #define IMCROPUI_H void setparams(int argc, char *argv[], struct imgarithparams *p); #endif gnuastro-0.2.33-8a3b/bin/arithmetic/ui.c0000644000175000017500000002551613001632537014610 00000000000000/********************************************************************* ImageArithmetic - Do arithmetic operations on images. ImageArithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include /* From Gnulib. */ #include /* Includes time.h and sys/time.h */ #include #include #include #include #include "main.h" #include "ui.h" /* Needs main.h */ #include "args.h" /* Needs main.h, includes argp.h. */ /* Set the file names of the places where the default parameters are put. */ #define CONFIG_FILE SPACK CONF_POSTFIX #define SYSCONFIG_FILE SYSCONFIG_DIR "/" CONFIG_FILE #define USERCONFIG_FILEEND USERCONFIG_DIR CONFIG_FILE #define CURDIRCONFIG_FILE CURDIRCONFIG_DIR CONFIG_FILE /**************************************************************/ /************** Options and parameters ***************/ /**************************************************************/ void readconfig(char *filename, struct imgarithparams *p) { FILE *fp; char *tokeephdu; size_t lineno=0, len=200; char *line, *name, *value; struct uiparams *up=&p->up; struct gal_commonparams *cp=&p->cp; char key='a'; /* Not used, just a place holder. */ /* When the file doesn't exist or can't be opened, it is ignored. It might be intentional, so there is no error. If a parameter is missing, it will be reported after all defaults are read. */ fp=fopen(filename, "r"); if (fp==NULL) return; /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); /* Read the tokens in the file: */ while(getline(&line, &len, fp) != -1) { /* Prepare the "name" and "value" strings, also set lineno. */ GAL_CONFIGFILES_START_READING_LINE; /* Inputs: */ if(strcmp(name, "hdu")==0) { gal_checkset_allocate_copy(value, &tokeephdu); gal_linkedlist_add_to_stll(&p->hdus, tokeephdu); } else if (strcmp(name, "mask")==0) gal_checkset_allocate_copy_set(value, &up->maskname, &up->masknameset); else if (strcmp(name, "mhdu")==0) gal_checkset_allocate_copy_set(value, &up->mhdu, &up->mhduset); /* Outputs */ else if(strcmp(name, "output")==0) gal_checkset_allocate_copy_set(value, &cp->output, &cp->outputset); else if(strcmp(name, "type")==0) { if(p->up.typeset) continue; gal_checkset_known_types(value, &p->type, filename, lineno); p->up.typeset=1; } /* Operating modes: */ /* Read options common to all programs */ GAL_CONFIGFILES_READ_COMMONOPTIONS_FROM_CONF else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s` not recognized.\n", name); } free(line); fclose(fp); } void printvalues(FILE *fp, struct imgarithparams *p) { struct uiparams *up=&p->up; struct gal_linkedlist_stll *hdu; struct gal_commonparams *cp=&p->cp; /* Print all the options that are set. Separate each group with a commented line explaining the options in that group. */ fprintf(fp, "\n# Input image(s):\n"); /* The order of the HDU linked list has already been corrected, so just print them as they were read in. */ for(hdu=p->hdus; hdu!=NULL; hdu=hdu->next) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("hdu", hdu->v); if(up->masknameset) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("mask", up->maskname); if(up->mhdu) GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("mhdu", up->mhdu); /* Output: */ fprintf(fp, "\n# Output:\n"); if(cp->outputset) fprintf(fp, CONF_SHOWFMT"%s\n", "output", cp->output); if(up->typeset) gal_configfiles_print_type(fp, p->type); /* For the operating mode, first put the macro to print the common options, then the (possible options particular to this program). */ fprintf(fp, "\n# Operating mode:\n"); GAL_CONFIGFILES_PRINT_COMMONOPTIONS; } /* Note that numthreads will be used automatically based on the configure time. Note that those options which are not mandatory must not be listed here. */ void checkifset(struct imgarithparams *p) { int intro=0; char comment[100]; size_t numhdus=gal_linkedlist_num_in_stll(p->hdus); /* Output parameters: */ if(p->up.typeset==0) GAL_CONFIGFILES_REPORT_NOTSET("type"); /* Make sure the number of HDUs is not less than the total number of FITS images. If there are more HDUs than there are FITS images, there is no problem (since they can come from the configuration files). It is expected that the user can call their own desired number of HDUs, and not rely on the configuration files too much, however, if the configuration file does contain some HDUs, then it will be a real pain to first clean the configuration file and then re-run arithmetic. The best way is to simply ignore them. */ if(numhdusnumfits) { sprintf(comment, "hdu (%zu FITS file(s), %zu HDUs)", p->numfits, numhdus); GAL_CONFIGFILES_REPORT_NOTSET(comment); } /* Report the (possibly) missing options. */ GAL_CONFIGFILES_END_OF_NOTSET_REPORT; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ /* The dash of a negative number will cause problems for the users, so to work properly we will go over all the options/arguments and if any one starts with a dash and is followed by a number, then the dash is replaced by NEGDASHREPLACE. */ void dashtonegchar(int argc, char *argv[]) { size_t i; for(i=0;inumfits=0; /* Go through all the tokens and do the job(s). */ for(token=p->tokens; token!=NULL; token=token->next) { if(gal_fits_name_is_fits(token->v)) ++p->numfits; else if(token->v[0]==NEGDASHREPLACE && isdigit(token->v[1]) ) token->v[0]='-'; } } /* Standard sanity checks. */ void sanitycheck(struct imgarithparams *p) { struct gal_linkedlist_stll *token; /* Set the output file name (if any is needed). Note that since the lists are already reversed, the first FITS file encountered, is the first FITS file given by teh user. Also, notet that these file name operations are only necessary for the first FITS file in the token list. */ for(token=p->tokens; token!=NULL; token=token->next) if(gal_fits_name_is_fits(token->v)) { /* Set the p->up.maskname accordingly: */ gal_fits_file_or_ext_name(token->v, p->cp.hdu, p->up.masknameset, &p->up.maskname, p->up.mhdu, p->up.mhduset, "mask"); /* Set the name of the output file: */ if(p->cp.outputset) gal_checkset_check_remove_file(p->cp.output, p->cp.dontdelete); else gal_checkset_automatic_output(token->v, "_arith.fits", p->cp.removedirinfo, p->cp.dontdelete, &p->cp.output); /* These were only necessary for the first FITS file in the tokens, so break out of the loop. */ break; } } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void setparams(int argc, char *argv[], struct imgarithparams *p) { struct gal_commonparams *cp=&p->cp; /* Set the non-zero initial values, the structure was initialized to have a zero value for all elements. */ cp->spack = SPACK; cp->verb = 1; cp->numthreads = num_processors(NPROC_CURRENT); cp->removedirinfo = 1; p->hdus = NULL; p->tokens = NULL; p->up.maskname = NULL; /* The hyphen of a negative number can be confused with a dash, so we will temporarily replace such hyphens with other characters. */ dashtonegchar(argc, argv); /* Read the arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Revert the conversion of the hyphen above back to the original character. */ negchartodashcountfits(p); /* Add the user default values and save them if asked. */ GAL_CONFIGFILES_CHECK_SET_CONFIG; /* The inputs are put in a lastin-firstout (simple) linked list, so change them to the correct order so the order we pop a node is the same order that the user input a value. */ gal_linkedlist_reverse_stll(&p->hdus); gal_linkedlist_reverse_stll(&p->tokens); /* Check if all the required parameters are set. */ checkifset(p); /* Print the values for each parameter. */ if(cp->printparams) GAL_CONFIGFILES_REPORT_PARAMETERS_SET; /* Do a sanity check. */ sanitycheck(p); } gnuastro-0.2.33-8a3b/bin/arithmetic/cite.h0000644000175000017500000000317112750745735015134 00000000000000/********************************************************************* Arithmetic - Do arithmetic operations on images. Arithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef CITE_H #define CITE_H #define ARITHMETICBIBTEX "" #define PRINTCITEABORT { \ printf("\nWe hope %s has been useful for your research.\n" \ "Citations are vital for the continued work on %s.\n" \ "Thank you for citing it in your research paper.\n" \ "\nPlease cite as \"%s\":\n\n%s\n\n%s", \ SPACK_NAME, SPACK_NAME, SPACK_STRING, \ GAL_STRINGS_MAIN_BIBTEX, ARITHMETICBIBTEX); \ exit(EXIT_SUCCESS); \ } #endif gnuastro-0.2.33-8a3b/bin/arithmetic/main.h0000644000175000017500000000753412776216523015137 00000000000000/********************************************************************* ImageArithmetic - Do arithmetic operations on images. ImageArithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include #include #include /* Progarm name macros: */ #define SPACK "astarithmetic" /* Subpackage executable name. */ #define SPACK_NAME "Arithmetic" /* Subpackage full name. */ #define SPACK_STRING SPACK_NAME" ("PACKAGE_NAME") "PACKAGE_VERSION /* Do not use the main commonargs.h option reader for the --hdu option. */ #define NOTCOMMONHDU 1 /* Constants: */ #define NEGDASHREPLACE 11 /* A vertical tab (ASCII=11) for negative dash */ #define NOOPTARRAY NULL #define NOOPTNUMBER NAN #define NOOPTFILENAME "" /* The operands can be in three ways: 1. A file name which is not read yet. When inactive, NOOPTFILENAME. 2. A number which is not used yet. When inactive, NOOPTNUMBER. 3. An array (operator output). When inactive, NOOPTARRAY. In every node of the operand linked list, only one of these should be active. The other two should be inactive. Otherwise it will be a bug and will cause problems. All the operands operate on this premise. */ struct operand { char *filename; char *hdu; double number; double *array; struct operand *next; }; struct uiparams { char *maskname; /* Name of mask image. */ char *mhdu; /* Mask image HDU. */ int typeset; int masknameset; int masknameallocated; int mhduset; }; struct imgarithparams { /* Other structures: */ struct uiparams up; /* User interface parameters. */ struct gal_commonparams cp; /* Common parameters. */ /* Input: */ struct gal_linkedlist_stll *hdus; /* List of all given HDU strings. */ struct gal_linkedlist_stll *tokens; /* List of all arithmetic tokens. */ float *array; /* Main array to keep results. */ float *tmp; /* Secondary array for temporary reading. */ size_t numfits; /* Total number of input FITS images. */ size_t addcounter; /* The number of FITS images added. */ size_t popcounter; /* The number of FITS images popped. */ size_t s0; /* Length of image along first C axis. */ size_t s1; /* Length of image along second C axis. */ int nwcs; /* The number of WCS coordinates. */ struct wcsprm *wcs; /* The WCS structure. */ int anyblank; /* If there are blank pixels in the image. */ /* Output: */ int type; /* User's desired output bixpix value. */ /* Operating mode: */ /* Internal: */ struct operand *operands; /* The operands linked list. */ time_t rawtime; /* Starting time of the program. */ }; #endif gnuastro-0.2.33-8a3b/bin/arithmetic/main.c0000644000175000017500000000311212774155622015116 00000000000000/********************************************************************* ImageArithmetic - Do arithmetic operations on images. ImageArithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include /* Includes time.h and sys/time.h */ #include "main.h" #include "ui.h" /* needs main.h. */ #include "arithmetic.h" /* needs main.h. */ int main (int argc, char *argv[]) { struct timeval t1; struct imgarithparams p={{0}, {0}, 0}; /* Set the starting time. */ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ setparams(argc, argv, &p); /* Run MakeProfiles */ imgarith(&p); /* Return successfully.*/ return 0; } gnuastro-0.2.33-8a3b/bin/arithmetic/Makefile.in0000644000175000017500000017263513004464626016106 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. 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BITSIZEOF_WINT_T = @BITSIZEOF_WINT_T@ CC = @CC@ CCDEPMODE = @CCDEPMODE@ CFLAGS = @CFLAGS@ CPP = @CPP@ CPPFLAGS = @CPPFLAGS@ CXX = @CXX@ CXXCPP = @CXXCPP@ CXXDEPMODE = @CXXDEPMODE@ CXXFLAGS = @CXXFLAGS@ CYGPATH_W = @CYGPATH_W@ DEFS = @DEFS@ DEPDIR = @DEPDIR@ DLLTOOL = @DLLTOOL@ DSYMUTIL = @DSYMUTIL@ DUMPBIN = @DUMPBIN@ ECHO_C = @ECHO_C@ ECHO_N = @ECHO_N@ ECHO_T = @ECHO_T@ EGREP = @EGREP@ EMULTIHOP_HIDDEN = @EMULTIHOP_HIDDEN@ EMULTIHOP_VALUE = @EMULTIHOP_VALUE@ ENOLINK_HIDDEN = @ENOLINK_HIDDEN@ ENOLINK_VALUE = @ENOLINK_VALUE@ EOVERFLOW_HIDDEN = @EOVERFLOW_HIDDEN@ EOVERFLOW_VALUE = @EOVERFLOW_VALUE@ ERRNO_H = @ERRNO_H@ EXEEXT = @EXEEXT@ FGREP = @FGREP@ FLOAT_H = @FLOAT_H@ GAL_LT_VERSION = @GAL_LT_VERSION@ GETOPT_H = @GETOPT_H@ GLIBC21 = @GLIBC21@ GNULIB_ACOSF = @GNULIB_ACOSF@ GNULIB_ACOSL = @GNULIB_ACOSL@ GNULIB_ASINF = @GNULIB_ASINF@ GNULIB_ASINL = @GNULIB_ASINL@ GNULIB_ATAN2F = @GNULIB_ATAN2F@ GNULIB_ATANF = @GNULIB_ATANF@ GNULIB_ATANL = @GNULIB_ATANL@ GNULIB_ATOLL = @GNULIB_ATOLL@ GNULIB_BTOWC = @GNULIB_BTOWC@ GNULIB_CALLOC_POSIX = @GNULIB_CALLOC_POSIX@ GNULIB_CANONICALIZE_FILE_NAME = @GNULIB_CANONICALIZE_FILE_NAME@ GNULIB_CBRT = @GNULIB_CBRT@ GNULIB_CBRTF = @GNULIB_CBRTF@ GNULIB_CBRTL = @GNULIB_CBRTL@ GNULIB_CEIL = @GNULIB_CEIL@ GNULIB_CEILF = @GNULIB_CEILF@ GNULIB_CEILL = @GNULIB_CEILL@ GNULIB_CHDIR = @GNULIB_CHDIR@ GNULIB_CHOWN = @GNULIB_CHOWN@ GNULIB_CLOSE = @GNULIB_CLOSE@ GNULIB_COPYSIGN = @GNULIB_COPYSIGN@ GNULIB_COPYSIGNF = @GNULIB_COPYSIGNF@ GNULIB_COPYSIGNL = @GNULIB_COPYSIGNL@ GNULIB_COSF = @GNULIB_COSF@ GNULIB_COSHF = @GNULIB_COSHF@ GNULIB_COSL = @GNULIB_COSL@ GNULIB_DPRINTF = @GNULIB_DPRINTF@ GNULIB_DUP = @GNULIB_DUP@ GNULIB_DUP2 = @GNULIB_DUP2@ GNULIB_DUP3 = @GNULIB_DUP3@ GNULIB_DUPLOCALE = @GNULIB_DUPLOCALE@ GNULIB_ENVIRON = @GNULIB_ENVIRON@ GNULIB_EUIDACCESS = @GNULIB_EUIDACCESS@ GNULIB_EXP2 = @GNULIB_EXP2@ GNULIB_EXP2F = @GNULIB_EXP2F@ GNULIB_EXP2L = @GNULIB_EXP2L@ GNULIB_EXPF = @GNULIB_EXPF@ GNULIB_EXPL = @GNULIB_EXPL@ GNULIB_EXPM1 = @GNULIB_EXPM1@ GNULIB_EXPM1F = @GNULIB_EXPM1F@ GNULIB_EXPM1L = @GNULIB_EXPM1L@ GNULIB_FABSF = @GNULIB_FABSF@ GNULIB_FABSL = @GNULIB_FABSL@ GNULIB_FACCESSAT = @GNULIB_FACCESSAT@ GNULIB_FCHDIR = @GNULIB_FCHDIR@ GNULIB_FCHMODAT = @GNULIB_FCHMODAT@ GNULIB_FCHOWNAT = @GNULIB_FCHOWNAT@ GNULIB_FCLOSE = @GNULIB_FCLOSE@ GNULIB_FCNTL = @GNULIB_FCNTL@ GNULIB_FDATASYNC = @GNULIB_FDATASYNC@ GNULIB_FDOPEN = @GNULIB_FDOPEN@ GNULIB_FFLUSH = @GNULIB_FFLUSH@ GNULIB_FFS = @GNULIB_FFS@ GNULIB_FFSL = @GNULIB_FFSL@ GNULIB_FFSLL = @GNULIB_FFSLL@ GNULIB_FGETC = @GNULIB_FGETC@ GNULIB_FGETS = @GNULIB_FGETS@ GNULIB_FLOOR = @GNULIB_FLOOR@ GNULIB_FLOORF = @GNULIB_FLOORF@ GNULIB_FLOORL = @GNULIB_FLOORL@ GNULIB_FMA = @GNULIB_FMA@ GNULIB_FMAF = @GNULIB_FMAF@ GNULIB_FMAL = @GNULIB_FMAL@ GNULIB_FMOD = @GNULIB_FMOD@ GNULIB_FMODF = @GNULIB_FMODF@ GNULIB_FMODL = @GNULIB_FMODL@ GNULIB_FOPEN = @GNULIB_FOPEN@ GNULIB_FPRINTF = @GNULIB_FPRINTF@ GNULIB_FPRINTF_POSIX = @GNULIB_FPRINTF_POSIX@ GNULIB_FPURGE = @GNULIB_FPURGE@ GNULIB_FPUTC = @GNULIB_FPUTC@ GNULIB_FPUTS = @GNULIB_FPUTS@ GNULIB_FREAD = @GNULIB_FREAD@ GNULIB_FREOPEN = @GNULIB_FREOPEN@ GNULIB_FREXP = @GNULIB_FREXP@ GNULIB_FREXPF = @GNULIB_FREXPF@ GNULIB_FREXPL = @GNULIB_FREXPL@ GNULIB_FSCANF = @GNULIB_FSCANF@ GNULIB_FSEEK = @GNULIB_FSEEK@ GNULIB_FSEEKO = @GNULIB_FSEEKO@ GNULIB_FSTAT = @GNULIB_FSTAT@ GNULIB_FSTATAT = @GNULIB_FSTATAT@ GNULIB_FSYNC = @GNULIB_FSYNC@ GNULIB_FTELL = @GNULIB_FTELL@ GNULIB_FTELLO = @GNULIB_FTELLO@ GNULIB_FTRUNCATE = @GNULIB_FTRUNCATE@ GNULIB_FUTIMENS = @GNULIB_FUTIMENS@ GNULIB_FWRITE = @GNULIB_FWRITE@ GNULIB_GETC = @GNULIB_GETC@ GNULIB_GETCHAR = @GNULIB_GETCHAR@ GNULIB_GETCWD = @GNULIB_GETCWD@ GNULIB_GETDELIM = @GNULIB_GETDELIM@ GNULIB_GETDOMAINNAME = @GNULIB_GETDOMAINNAME@ GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ 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uninstall-dist_sysconfDATA .MAKE: install-am install-strip .PHONY: CTAGS GTAGS TAGS all all-am check check-am clean \ clean-binPROGRAMS clean-generic clean-libtool cscopelist-am \ ctags ctags-am distclean distclean-compile distclean-generic \ distclean-libtool distclean-tags distdir dvi dvi-am html \ html-am info info-am install install-am install-binPROGRAMS \ install-data install-data-am install-dist_sysconfDATA \ install-dvi install-dvi-am install-exec install-exec-am \ install-html install-html-am install-info install-info-am \ install-man install-pdf install-pdf-am install-ps \ install-ps-am install-strip installcheck installcheck-am \ installdirs maintainer-clean maintainer-clean-generic \ mostlyclean mostlyclean-compile mostlyclean-generic \ mostlyclean-libtool pdf pdf-am ps ps-am tags tags-am uninstall \ uninstall-am uninstall-binPROGRAMS uninstall-dist_sysconfDATA .PRECIOUS: Makefile # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: gnuastro-0.2.33-8a3b/bin/arithmetic/astarithmetic.conf0000644000175000017500000000156712760077036017547 00000000000000# Default parameters (System) for ImageArithmetic. # ImageArithmetic is part of GNU Astronomy Utitlies. # # Use the long option name of each paramter followed by # a value. The name and value should be separated by # atleast one of the following charaacters: # space, `,`, `=` or `:` # # Run with `--help` option or read the manual for a full # explanation of what each option means. # # NOTE I: All counting is from zero, not one. # NOTE II: Lines starting with `#` are ignored. # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Input image: hdu 0 hdu 0 hdu 0 hdu 0 hdu 0 hdu 0 hdu 0 # Output: type float gnuastro-0.2.33-8a3b/bin/arithmetic/Makefile.am0000644000175000017500000000272112765246733016073 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. NOTE: $(top_srcdir)/bootstrapped/lib is only necessary ## for internally compiled utilities and libraries. It must not be included ## during the tests since the bootstrapped libraries are not installed. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Utility and its sources bin_PROGRAMS = astarithmetic astarithmetic_SOURCES = main.c main.h cite.h ui.c ui.h args.h \ arithmetic.c arithmetic.h astarithmetic_LDADD = $(top_builddir)/bootstrapped/lib/libgnu.la \ -lgnuastro ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astarithmetic.conf gnuastro-0.2.33-8a3b/lib/0000755000175000017500000000000013004464724011747 500000000000000gnuastro-0.2.33-8a3b/lib/timing.h0000644000175000017500000000374012772171231013332 00000000000000/********************************************************************* Functions to report timing in verbose mode. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_TIMING_H__ #define __GAL_TIMING_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ #define GAL_TIMING_VERB_MSG_LENGTH_V 45 #define GAL_TIMING_VERB_MSG_LENGTH_T "45" #define GAL_TIMING_VERB_MSG_LENGTHS_2_V 65 #define GAL_TIMING_VERB_MSG_LENGTHS_2_T "65" unsigned long int gal_timing_time_based_rng_seed(); void gal_timing_report(struct timeval *t1, char *jobname, size_t level); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_TIMING_H__ */ gnuastro-0.2.33-8a3b/lib/neighbors.h0000644000175000017500000001667312772171231014034 00000000000000/********************************************************************* neighbors.h -- Find the neighbours around a pixel. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_NEIGHBORS_H__ #define __GAL_NEIGHBORS_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* These macros can be put any where you want to know the neighbors of an index, the important values that have to be declared and defined before this macro are: Inputs: ind : Pointer to the index being considered. (is0, is1) : Input image number of rows and columns. (x0,y0) : The bottom left corner of image or mesh box (included). (x1,y1) : The Top right corner of image or mesh box (not included). Outputs: numngb : Number of filled neighbors. *ngb : Array keeping the neighbours indexs (allocated outside). */ #define GAL_NEIGHBORS_FILL_4_REGION { \ numngb=0; \ if (*ind/is1!=x0 ) ngb[numngb++]=*ind-is1; \ if (*ind/is1!=x1-1) ngb[numngb++]=*ind+is1; \ if (*ind%is1!=y0 ) ngb[numngb++]=*ind-1; \ if (*ind%is1!=y1-1) ngb[numngb++]=*ind+1; \ } #define GAL_NEIGHBORS_FILL_4_ALLIMG { \ numngb=0; \ if (*ind/is1!=0 ) ngb[numngb++]=*ind-is1; \ if (*ind/is1!=is0-1) ngb[numngb++]=*ind+is1; \ if (*ind%is1!=0 ) ngb[numngb++]=*ind-1; \ if (*ind%is1!=is1-1) ngb[numngb++]=*ind+1; \ } #define GAL_NEIGHBORS_FILL_8_REGION { \ unsigned char bl=0, br=0, tl=0, tr=0; \ numngb=0; \ if (*ind/is1!=x0 ) {ngb[numngb++]=*ind-is1; ++bl; ++br;} \ if (*ind/is1!=x1-1) {ngb[numngb++]=*ind+is1; ++tl; ++tr;} \ if (*ind%is1!=y0 ) {ngb[numngb++]=*ind-1; ++bl; ++tl;} \ if (*ind%is1!=y1-1) {ngb[numngb++]=*ind+1; ++tr; ++br;} \ if (numngb==4) \ { \ numngb=8; \ ngb[4]=*ind-is1-1; ngb[5]=*ind-is1+1; \ ngb[6]=*ind+is1-1; ngb[7]=*ind+is1+1; \ } \ else \ { \ if(bl==2) ngb[numngb++]=*ind-is1-1; \ if(br==2) ngb[numngb++]=*ind-is1+1; \ if(tl==2) ngb[numngb++]=*ind+is1-1; \ if(tr==2) ngb[numngb++]=*ind+is1+1; \ } \ } #define GAL_NEIGHBORS_FILL_8_ALLIMG { \ unsigned char bl=0, br=0, tl=0, tr=0; \ numngb=0; \ if (*ind/is1!=0 ) {ngb[numngb++]=*ind-is1; ++bl; ++br;} \ if (*ind/is1!=is0-1 ) {ngb[numngb++]=*ind+is1; ++tl; ++tr;} \ if (*ind%is1!=0 ) {ngb[numngb++]=*ind-1; ++bl; ++tl;} \ if (*ind%is1!=is1-1 ) {ngb[numngb++]=*ind+1; ++tr; ++br;} \ if (numngb==4) \ { \ numngb=8; \ ngb[4]=*ind-is1-1; ngb[5]=*ind-is1+1; \ ngb[6]=*ind+is1-1; ngb[7]=*ind+is1+1; \ } \ else \ { \ if(bl==2) ngb[numngb++]=*ind-is1-1; \ if(br==2) ngb[numngb++]=*ind-is1+1; \ if(tl==2) ngb[numngb++]=*ind+is1-1; \ if(tr==2) ngb[numngb++]=*ind+is1+1; \ } \ } #define GAL_NEIGHBORS_FILL_8_ALLIMG_IJ { \ unsigned char bl=0, br=0, tl=0, tr=0; \ numngb=0; \ if (i!=0 ) {ngb[numngb++]=(i-1)*is1+j; ++bl; ++br;} \ if (i!=is0-1 ) {ngb[numngb++]=(i+1)*is1+j; ++tl; ++tr;} \ if (j!=0 ) {ngb[numngb++]=i*is1+j-1; ++bl; ++tl;} \ if (j!=is1-1 ) {ngb[numngb++]=i*is1+j+1; ++tr; ++br;} \ if (numngb==4) \ { \ numngb=8; \ ngb[4]=(i-1)*is1+j-1; ngb[5]=(i-1)*is1+j+1; \ ngb[6]=(i+1)*is1+j-1; ngb[7]=(i+1)*is1+j+1; \ } \ else \ { \ if(bl==2) ngb[numngb++]=(i-1)*is1+j-1; \ if(br==2) ngb[numngb++]=(i-1)*is1+j+1; \ if(tl==2) ngb[numngb++]=(i+1)*is1+j-1; \ if(tr==2) ngb[numngb++]=(i+1)*is1+j+1; \ } \ } __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_NEIGHBORS_H__ */ gnuastro-0.2.33-8a3b/lib/mode.h0000644000175000017500000000303712772171231012766 00000000000000/********************************************************************* mode -- Find the mode of a distribution. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __MODE_H__ #define __MODE_H__ #include #define MODE_GOLDEN_RATIO 1.618034f #define MODE_TWO_TAKE_GOLDEN_RATIO 0.38197f #define MODE_MIRROR_IS_ABOVE_RESULT (size_t)(-1) size_t mirrormaxdiff(float *a, size_t size, size_t m, size_t numcheck, size_t interval, size_t stdm); void modesymmetricity(float *a, size_t size, size_t mi, float errorstdm, float *sym); size_t modegoldenselection(struct gal_statistics_mode_params *mp); void makemirrored(float *in, size_t mi, float **outmirror, size_t *outsize); #endif gnuastro-0.2.33-8a3b/lib/fixedstringmacros.h0000644000175000017500000001102212772171231015566 00000000000000/********************************************************************* Fixed strings for use in all utilities. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_FIXEDSTRINGMACROS_H__ #define __GAL_FIXEDSTRINGMACROS_H__ #define GAL_STRINGS_SHORT_COPYRIGHT \ "Copyright (C) 2015-2016, Free Software Foundation, Inc." #define GAL_STRINGS_SHORT_LICENSE \ "License GPLv3+: GNU General public license version 3 or later." #define GAL_STRINGS_COPYRIGHT \ GAL_STRINGS_SHORT_COPYRIGHT"\n"GAL_STRINGS_SHORT_LICENSE"\n" \ "This is free software: you are free to change and redistribute " \ "it.\nThere is NO WARRANTY, to the extent permitted by law." \ #define GAL_STRINGS_TOP_HELP_INFO \ "\n"SPACK_NAME" is part of "PACKAGE_STRING".\n" /* This is fixed for all the packages. */ #define GAL_STRINGS_MORE_HELP_INFO \ "\nFor more information, please run any of the " \ "following commands. They will respectively show you the `Invoking " \ SPACK_NAME"' subsection, the complete `"SPACK_NAME"' section, or " \ "the full "PACKAGE_NAME" manual. In particular the first contains " \ "a very complete explanation of each option.\n\n" \ " info "SPACK"\n\n" \ " info "SPACK_NAME"\n\n" \ " info "PACKAGE_TARNAME"\n\n" \ "If you couldn't find your answer in the manual, you can get " \ "direct help from experienced Gnuastro users and developers. " \ "For more information, please run:\n\n" \ " info help-gnuastro\n\n" \ SPACK_NAME" options:" \ #define GAL_STRINGS_MAIN_BIBTEX \ "@ARTICLE{noisechisel,\n" \ " author = {{Akhlaghi}, M. and {Ichikawa}, T.},\n" \ " title = \"{Noise-based Detection and Segmentation of Nebulous " \ "Objects}\",\n" \ " journal = {\\apjs},\n" \ "archivePrefix = \"arXiv\",\n" \ " eprint = {1505.01664},\n" \ " primaryClass = \"astro-ph.IM\",\n" \ " keywords = {galaxies: irregular, galaxies: photometry, " \ "galaxies: structure, methods: data analysis, " \ "techniques: image processing, techniques: photometric},\n" \ " year = 2015,\n" \ " month = sep,\n" \ " volume = 220,\n" \ " eid = {1},\n" \ " pages = {1},\n" \ " doi = {10.1088/0067-0049/220/1/1},\n" \ " adsurl = {http://adsabs.harvard.edu/abs/2015ApJS..220....1A},\n" \ " adsnote = {Provided by the SAO/NASA Astrophysics Data System}\n" \ "}" /* This can be used in the end of error messages related to option values. */ #define GAL_STRINGS_HOW_TO_CHECK_VALUES \ " You can check all the input values with the `--printparams' " \ "(-P) option." #endif /* __GAL_FIXEDSTRINGMACROS_H__ */ gnuastro-0.2.33-8a3b/lib/configfiles.h0000644000175000017500000002777113001632540014334 00000000000000/********************************************************************* configfiles -- Read configuration files for each program. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_CONFIGFILES_H__ #define __GAL_CONFIGFILES_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /**************************************************************/ /************ Macros *************/ /**************************************************************/ /* Simple macros: */ #define GAL_CONFIGFILES_DELIMITERS " ,=:\t\n" #define GAL_CONFIGFILES_START_READING_LINE { \ ++lineno; \ if(*line=='#') continue; \ else gal_configfiles_read_name_value(line, filename, lineno, \ &name, &value); \ if(name==NULL && value==NULL) continue; \ } /* Functional macros: These are not actual functions, because they depend on functions that are different for different programs. So they have to be written into the functions with a macro. */ #define GAL_CONFIGFILES_SAVE_LOCAL_CONFIG(INDIR) { \ FILE *fp; \ char *outfilename, *command; \ fp=gal_configfiles_write_local_config_stop(INDIR, CONFIG_FILE, \ SPACK, SPACK_NAME, \ &outfilename); \ printvalues(fp, p); \ errno=0; \ if(fclose(fp)==-1) \ error(EXIT_FAILURE, errno, "%s", outfilename); \ command=gal_checkset_malloc_cat("cat ", outfilename); \ printf("Values saved in %s:\n\n", outfilename); \ if(system(command)) \ error(EXIT_FAILURE, 0, "the `%s` command could not be run or " \ "failed", command); \ free(outfilename); \ free(command); \ exit(EXIT_SUCCESS); \ } #define GAL_CONFIGFILES_CHECK_SET_CONFIG { \ char *userconfig_dir, *userconfig_file; \ \ readconfig(CURDIRCONFIG_FILE, p); \ if(cp->setdirconf) \ GAL_CONFIGFILES_SAVE_LOCAL_CONFIG(CURDIRCONFIG_DIR); \ if(cp->onlyversionset && strcmp(cp->onlyversion, PACKAGE_VERSION)) \ error(EXIT_FAILURE, 0, "you are currently running Gnuastro %s. " \ "However, this run should be with version `%s'.\n\n" \ "To resolve the situation, use the the '--onlyversion' " \ "option, either on the command-line or in a configuration " \ "file. For example, set it to `%s' by repeating the " \ "previous command with:\n\n" \ " --onlyversion=%s\n\n" \ "Alternatively, you can install Gnuastro %s.\n\n" \ "NOTE: If you didn't set this option on the command-line, " \ "it was probably intended for reproducability. If so, it " \ "is advised to install Gnuastro %s", \ PACKAGE_VERSION, cp->onlyversion, PACKAGE_VERSION, \ PACKAGE_VERSION, cp->onlyversion, cp->onlyversion); \ \ if(cp->onlydirconf==0) \ { \ userconfig_dir=gal_configfiles_add_home_dir(USERCONFIG_DIR); \ userconfig_file= \ gal_configfiles_add_home_dir(USERCONFIG_FILEEND); \ readconfig(userconfig_file, p); \ if(cp->setusrconf) \ GAL_CONFIGFILES_SAVE_LOCAL_CONFIG(userconfig_dir); \ readconfig(SYSCONFIG_FILE, p); \ free(userconfig_file); \ free(userconfig_dir); \ } \ } #define GAL_CONFIGFILES_REPORT_NOTSET(var_name) { \ if(intro==0) \ { \ fprintf(stderr, SPACK": Parameter(s) not set: `%s'", \ (var_name)); \ intro=1; \ } \ else \ fprintf(stderr, ", `%s'", (var_name)); \ } #define GAL_CONFIGFILES_END_OF_NOTSET_REPORT { \ if(intro) \ { \ char *userconfig_file; \ fprintf(stderr, ".\n\n"); \ fprintf(stderr, "You can assign values in the local, user or " \ "system wide default files. Otherwise you have to " \ "explicitly assign a value to them each time as a " \ "command-line option. See `%s --help` or `info %s` for "\ "more information.\n\n", SPACK, SPACK); \ userconfig_file= \ gal_configfiles_add_home_dir(USERCONFIG_FILEEND); \ fprintf(stderr, "Default files checked (existing or not):\n"); \ fprintf(stderr, " %s\n", CURDIRCONFIG_FILE); \ if(p->cp.onlydirconf==0) \ fprintf(stderr, " %s\n %s\n", userconfig_file, \ SYSCONFIG_FILE); \ free(userconfig_file); \ exit(EXIT_FAILURE); \ } \ } #define GAL_CONFIGFILES_REPORT_PARAMETERS_SET { \ fprintf(stdout, "# "SPACK_STRING"\n"); \ fprintf(stdout, "# Configured on "CONFIGDATE" at "CONFIGTIME"\n"); \ fprintf(stdout, "# Written on %s", ctime(&p->rawtime)); \ printvalues(stdout, p); \ exit(EXIT_SUCCESS); \ } /* Read the options that are common to all programs from the configuration file. Since these two checks are within an if-else structure, they should not be placed within an `{' and `}'. */ #define GAL_CONFIGFILES_READ_COMMONOPTIONS_FROM_CONF \ else if(strcmp(name, "numthreads")==0) \ { \ if(cp->numthreadsset) continue; \ gal_checkset_sizet_l_zero(value, &cp->numthreads, name, key, \ SPACK, filename, lineno); \ cp->numthreadsset=1; \ } \ else if(strcmp(name, "nolog")==0) \ { \ if(cp->nologset) continue; \ gal_checkset_int_zero_or_one(value, &cp->nolog, name, key, \ SPACK, filename, lineno); \ cp->nologset=1; \ } \ else if(strcmp(name, "onlydirconf")==0) \ { \ if(cp->onlydirconf==0) \ gal_checkset_int_zero_or_one(value, &cp->onlydirconf, name, \ key, SPACK, filename, lineno); \ } \ else if(strcmp(name, "onlyversion")==0) \ gal_checkset_allocate_copy_set(value, &cp->onlyversion, \ &cp->onlyversionset); \ /* Write common options: */ #define GAL_CONFIGFILES_PRINT_COMMONOPTIONS { \ if(cp->numthreadsset) \ fprintf(fp, CONF_SHOWFMT"%zu\n", "numthreads", p->cp.numthreads); \ if(cp->nologset) \ fprintf(fp, CONF_SHOWFMT"%d\n", "nolog", p->cp.nolog); \ if(cp->onlyversionset) \ GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE("onlyversion", \ cp->onlyversion); \ } /**************************************************************/ /************ Function declarations *************/ /**************************************************************/ char * gal_configfiles_add_home_dir(char *dir); void gal_configfiles_read_name_value(char *line, char *filename, size_t lineno, char **name, char **value); FILE * gal_configfiles_write_local_config_stop(char *indir, char *filename, char *spack, char *spack_name, char **outfilename); void gal_configfiles_print_type(FILE *fp, int bitpix); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_CONFIGFILES_H__ */ gnuastro-0.2.33-8a3b/lib/commonparams.h0000644000175000017500000000515012772171231014534 00000000000000/********************************************************************* Common parameters for all the utilities. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_COMMONPARAMS_H__ #define __GAL_COMMONPARAMS_H__ /* The structure keeping all the common parameters in gnuastro. This could be part of commonargs.h, but since main.h in all those programs will need this structure, there will be problems about the unused `commonargp` structure.*/ struct gal_commonparams { char *spack; /* Subpackage name. */ /* Input/Output: */ char *output; /* Directory containg output. */ char *hdu; /* Image extension. */ int dontdelete; /* ==1: Don't delete existing. */ int removedirinfo; /* ==1: Remove directory information. */ /* Operating modes: */ int verb; /* ==1: report steps. ==0 don't. */ int printparams; /* Only print the used values. */ int setdirconf; /* ==1: Set the current directory config. */ int setusrconf; /* ==1: Set the user default values. */ size_t numthreads; /* Number of threads to use. */ int onlydirconf; /* Only check current directory conf. file. */ char *onlyversion; /* The string of the requested version. */ int nolog; /* ==1: do not make a log file. */ /* Check: */ int numthreadsset; /* If the number of threads are set. */ int onlyversionset; /* If the only version option is set. */ int hduset; /* If the input image extension is set. */ int outputset; /* If the output is set. */ int nologset; /* If nolog is set. */ }; #endif gnuastro-0.2.33-8a3b/lib/commonargs.h0000644000175000017500000001361312774155746014227 00000000000000/********************************************************************* Argument parsing for options that are common to all programs. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_COMMONARGS_H__ #define __GAL_COMMONARGS_H__ #include #include #include #include #include #include #include /* These are separate in each package. */ #include "main.h" #include "cite.h" /* Fixed options for all the programs: Free letters (-V which is used by GNU is also removed): a b c d e f g i j k l m n p r s t u v w x y z A B C E F G H I J L M O Q R T U W X Y Z Used numbers <= 1003 You can use this above list to set short options for the different utilities. */ static struct argp_option gal_commonargs_options[] = { /* -1 is the code for operating modes: */ { "quiet", 'q', 0, 0, "Only report errors, remain quiet about steps.", -1 }, { "printparams", 'P', 0, 0, "Print parameter values to be used and abort.", -1 }, { "setdirconf", 'S', 0, 0, "Set default values for this directory and abort.", -1 }, { "setusrconf", 'U', 0, 0, "Set default values for this user and abort.", -1 }, { "numthreads", 'N', "INT", 0, "Number of CPU threads to use.", -1 }, { "cite", 1000, 0, 0, "BibTeX citation for "SPACK_NAME".", -1 }, { "onlydirconf", 1001, 0, 0, "Only read current directory configuration file.", -1 }, { "onlyversion", 1002, "STR", 0, "Only run if the program version is this.", -1 }, { "nolog", 1003, 0, 0, "No log file for programs which make one.", -1 }, /* 1 is the code for inputs. Some utilities might need their own HDU option reader, if that is the case, then the NOTCOMMONHDU is defined in their main.h.*/ #ifndef NOTCOMMONHDU { "hdu", 'h', "STR", 0, "Extension name or number of input data.", 1 }, #endif /* 2 is the code for output in all programs: */ { "output", 'o', "STR", 0, "Output file or directory name.", 2 }, { "dontdelete", 'D', 0, 0, "Don't delete output if it exists.", 2 }, { "keepinputdir", 'K', 0, 0, "Do not remove input's dir info for output.", 2 }, {0} }; static error_t gal_checkset_commonargs_cparse_opt(int key, char *arg, struct argp_state *state) { /* Save the arguments structure: */ struct gal_commonparams *cp=state->input; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); switch(key) { /* Operating modes: */ case 'q': cp->verb=0; break; case 'P': cp->printparams=1; break; case 'S': cp->setdirconf=1; break; case 'U': cp->setusrconf=1; break; case 'N': gal_checkset_sizet_l_zero(arg, &cp->numthreads, "numthreads", key, cp->spack, NULL, 0); cp->numthreadsset=1; break; case 1000: PRINTCITEABORT; break; case 1001: cp->onlydirconf=1; break; case 1002: cp->onlyversion=arg; cp->onlyversionset=1; break; case 1003: cp->nolog=1; cp->nologset=1; break; /* Input/output: */ case 'h': gal_checkset_allocate_copy_set(arg, &cp->hdu, &cp->hduset); break; case 'o': gal_checkset_allocate_copy_set(arg, &cp->output, &cp->outputset); break; case 'D': cp->dontdelete=1; break; case 'K': cp->removedirinfo=0; break; /* Once finished: */ case ARGP_KEY_END: if(cp->setdirconf && cp->setusrconf) error(EXIT_FAILURE, 0, "only one of `--setusrconf` or " "`--setdirconf` may be set in each run. You have asked " "for both"); break; /* If the argument is not known. */ default: return ARGP_ERR_UNKNOWN; } return 0; } static struct argp commonargp = {gal_commonargs_options, gal_checkset_commonargs_cparse_opt, NULL, NULL, NULL, NULL, NULL}; #endif /* __GAL_COMMONARGS_H__ */ gnuastro-0.2.33-8a3b/lib/checkset.h0000644000175000017500000002043113001632540013617 00000000000000/********************************************************************* Functions to check and set command line argument values and files. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_CHECKSET_H__ #define __GAL_CHECKSET_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /**************************************************************/ /********* Macros **************/ /**************************************************************/ /* Check if the column number is within the boundaries of a catalog. */ #define GAL_CHECKSET_CHECK_COL_NUM_IN_CAT(INCOL,NAME) { \ if( (INCOL) >= p->cs1 ) \ error(EXIT_FAILURE, 0, "%s only has %zu columns while you " \ "have requested column %zu (counting from zero) for " \ "`--%s`", p->up.catname, p->cs1, (INCOL), (NAME)); \ } /* Check both the column number and that the values in the column are finitte numbers (not infinities or NAN). */ #define GAL_CHECKSET_CHECK_COL_IN_CAT(INCOL,NAME) { \ size_t i; \ \ if( (INCOL) >= p->cs1 ) \ error(EXIT_FAILURE, 0, "%s only has %zu columns while you " \ "have requested column %zu (counting from zero) for " \ "`--%s`", p->up.catname, p->cs1, (INCOL), (NAME)); \ \ for(i=0;ics0;++i) \ if( !isfinite(p->cat[i*p->cs1+(INCOL)]) ) \ error(EXIT_FAILURE, 0, "%s: column %zu (--%s) in row %zu " \ "could not be read as a number. See %s. Note that " \ "counting starts from zero", \ p->up.catname, (INCOL), (NAME), i, GAL_TXTARRAY_LOG); \ } #define GAL_CHECKSET_PRINT_STRING_MAYBE_WITH_SPACE(name,string) { \ if(gal_checkset_string_has_space(string)) \ fprintf(fp, CONF_SHOWFMT"\"%s\"\n", name, string); \ else \ fprintf(fp, CONF_SHOWFMT"%s\n", name, string); \ } /**************************************************************** ************ Check and convert strings ***************** ****************************************************************/ int gal_checkset_str_is_double(char *string, double *out); /**************************************************************/ /********* Read arguments and check their values **************/ /**************************************************************/ void gal_checkset_int_zero_or_one(char *optarg, int *var, char *lo, char so, char* spack, char *filename, size_t lineno); void gal_checkset_int_4_or_8(char *optarg, int *var, char *lo, char so, char *spack, char *filename, size_t lineno); void gal_checkset_int_el_zero(char *optarg, int *var, char *lo, char so, char *spack, char *filename, size_t lineno); void gal_checkset_int_l_zero(char *optarg, int *var, char *lo, char so, char *spack, char *filename, size_t lineno); void gal_checkset_int_smaller_equal_to(char *optarg, int *var, char *lo, char so, char *spack, char *filename, size_t lineno, long maxvalue); void gal_checkset_long_el_zero(char *optarg, long *var, char *lo, char so, char *spack, char *filename, size_t lineno); void gal_checkset_any_long(char *optarg, long *var, char *lo, char so, char *spack, char *filename, size_t lineno); void gal_checkset_sizet_el_zero(char *optarg, size_t *var, char *lo, char so, char *spack, char *filename, size_t lineno); void gal_checkset_sizet_l_zero(char *optarg, size_t *var, char *lo, char so, char *spack, char *filename, size_t lineno); void gal_checkset_sizet_p_odd(char *optarg, size_t *var, char *lo, char so, char* spack, char *filename, size_t lineno); void gal_checkset_float_l_0(char *optarg, float *var, char *lo, char so, char *spack, char *filename, size_t lineno); void gal_checkset_float_l_0_s_1(char *optarg, float *var, char *lo, char so, char *spack, char *filename, size_t lineno); void gal_checkset_any_float(char *optarg, float *var, char *lo, char so, char *spack, char *filename, size_t lineno); void gal_checkset_double_l_0(char *optarg, double *var, char *lo, char so, char *spack, char *filename, size_t lineno); void gal_checkset_double_el_0(char *optarg, double *var, char *lo, char so, char* spack, char *filename, size_t lineno); void gal_checkset_double_l_value(char *optarg, double *var, char *lo, char so, char* spack, double value, char *filename, size_t lineno); void gal_checkset_any_double(char *optarg, double *var, char *lo, char so, char *spack, char *filename, size_t lineno); /**************************************************************/ /********** Check fixed strings ************/ /**************************************************************/ void gal_checkset_known_types(char *optarg, int *bitpix, char *filename, size_t lineno); /**************************************************************/ /********** My String functions: ************/ /**************************************************************/ int gal_checkset_string_has_space(char *in); char * gal_checkset_malloc_cat(char *inname, char *toappend); void gal_checkset_allocate_copy(char *arg, char **copy); void gal_checkset_allocate_copy_set(char *arg, char **copy, int *set); /**************************************************************/ /********** Set file names and check if they exist ************/ /**************************************************************/ void gal_checkset_check_file(char *filename); int gal_checkset_check_file_report(char *filename); void gal_checkset_check_remove_file(char *filename, int dontdelete); int gal_checkset_dir_0_file_1(char *name, int dontdelete); void gal_checkset_automatic_output(char *inname, char *suffix, int removedirinfo, int dontdelete, char **outname); char * gal_checkset_dir_part(char *input); char * gal_checkset_not_dir_part(char *input); void gal_checkset_check_dir_write_add_slash(char **dirname); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_CHECKSET_H__ */ gnuastro-0.2.33-8a3b/lib/gnuastro.h.in0000644000175000017500000000355613001632540014306 00000000000000/********************************************************************* Functions dealing with general aspects of all Gnuastro. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_GNUASTRO_H__ #define __GAL_GNUASTRO_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* Macros. In gnuastro.h.in, the values in `@' --- `@'', will be replaced with installation specific values. */ #define GAL_GNUASTRO_VERSION "@VERSION@" #define GAL_GNUASTRO_HAVE_LIBGIT2 @HAVE_LIBGIT2@ #define GAL_GNUASTRO_HAVE_PTHREAD_BARRIER @HAVE_PTHREAD_BARRIER@ /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_GNUASTRO_H__ */ gnuastro-0.2.33-8a3b/lib/gnuastro.pc.in0000644000175000017500000000044412765554423014475 00000000000000prefix=@prefix@ exec_prefix=@exec_prefix@ libdir=@libdir@ includedir=@includedir@ Name: Gnuastro Description: GNU Astronomy Utilities URL: https://www.gnu.org/software/gnuastro/ Version: @VERSION@ Requires.private: wcs cfitsio gsl Cflags: -I${includedir} Libs: -L${libdir} -lgnuastro @LIBS@ gnuastro-0.2.33-8a3b/lib/wcs.c0000644000175000017500000001312313001632540012615 00000000000000/********************************************************************* Functions to that only use WCSLIB functionality. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include /**************************************************************/ /********** XY to RADEC ************/ /**************************************************************/ /* Use the X and Y columns in a larger array to fill the RA and Dec columns in that same array. `xy' points to the first element in the X column and `radec' points to the first element in the RA column. The columns for Y and Dec have to be immediately after X and RA. It appears that WCSLIB can only deal with static allocation. At least in its tests it only uses static allocation. I tried dynamic allocation, but it didn't work. So I can't use the vector functionalities of WCSLIB and have to translate each point separately. */ void gal_wcs_xy_array_to_radec(struct wcsprm *wcs, double *xy, double *radec, size_t number, size_t stride) { size_t i; double imgcrd[2], phi, theta; int stat, status=0, ncoord=1, nelem=2; for(i=0;i (%f, %f)\n", xy[i*stride], xy[i*stride+1], radec[i*stride], radec[i*stride+1]); */ } } } /* Similar to the gal_wcs_xyarray_to_radec, but the reverse: to convert an array of RA-Dec to X-Y. */ void gal_wcs_radec_array_to_xy(struct wcsprm *wcs, double *radec, double *xy, size_t number, size_t stride) { size_t i; double imgcrd[2], phi, theta; int stat, status=0, ncoord=1, nelem=2; for(i=0;i (%f, %f)\n", radec[i*stride], radec[i*stride+1], xy[i*stride], xy[i*stride+1]); */ } } } /* The distance (along a great circle) on a sphere between two points is calculated here. Since the pixel sides are usually very small, we won't be using the direct formula: cos(distance)=sin(d1)*sin(d2)+cos(d1)*cos(d2)*cos(r1-r2) We will be using the haversine formula which better considering floating point errors (from Wikipedia:) sin^2(distance)/2=sin^2( (d1-d2)/2 )+cos(d1)*cos(d2)*sin^2( (r1-r2)/2 ) Inputs and outputs are all in degrees. */ double gal_wcs_angular_distance_deg(double r1, double d1, double r2, double d2) { /* Convert degrees to radians. */ double r1r=r1*M_PI/180, d1r=d1*M_PI/180; double r2r=r2*M_PI/180, d2r=d2*M_PI/180; /* To make things easier to read: */ double a=sin( (d1r-d2r)/2 ); double b=sin( (r1r-r2r)/2 ); /* Return the result: */ return 2*asin( sqrt( a*a + cos(d1r)*cos(d2r)*b*b) ) * 180/M_PI; } /* Return the pixel scale of the image in both dimentions in degrees. */ void gal_wcs_pixel_scale_deg(struct wcsprm *wcs, double *dx, double *dy) { double radec[6], xy[]={0,0,1,0,0,1}; /* Get the RA and Dec of the bottom left, bottom right and top left sides of the first pixel in the image. */ gal_wcs_xy_array_to_radec(wcs, xy, radec, 3, 2); /* Calculate the distances and convert back to degrees: */ *dx = gal_wcs_angular_distance_deg(radec[0], radec[1], radec[2], radec[3]); *dy = gal_wcs_angular_distance_deg(radec[0], radec[1], radec[4], radec[5]); } /* Report the arcsec^2 area of the pixels in the image based on the WCS information in that image. We first use the angular distance of two edges of one pixel in radians. Then the radians are multiplied to give stradians and finally, the stradians are converted to arcsec^2. */ double gal_wcs_pixel_area_arcsec2(struct wcsprm *wcs) { double dx, dy; /* Get the pixel scales along each axis in degrees. */ gal_wcs_pixel_scale_deg(wcs, &dx, &dy); /* Return the result */ return dx * dy * 3600.0f * 3600.0f; } gnuastro-0.2.33-8a3b/lib/txtarray.c0000644000175000017500000003047213001632540013705 00000000000000/********************************************************************* txtarray -- Convert a text file table to a C array. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include /* Internal macros */ #define GAL_TXTARRAY_FMT_LENGTH 50 #define GAL_TXTARRAY_DELIMITERS " ,\t\n" /**********************************************************************/ /***************** Read a text table *********************/ /**********************************************************************/ static void txttablesize(char *filename, size_t *outs0, size_t *outs1) { FILE *fp; size_t len=200, s0, s1; char *line, *firsttoken; /* Initialize the sizes any way. */ s0=s1=0; /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); /* Open the file: */ errno=0; fp=fopen(filename, "r"); if(fp==NULL) error(EXIT_FAILURE, errno, "%s", filename); while( getline(&line, &len, fp) != -1 ) { /* Read the first token: */ firsttoken=strtok(line, GAL_TXTARRAY_DELIMITERS); /* If there are no non-delimters in the line (can happen if the line is a blank line in the end of the file). */ if(firsttoken==NULL) continue; /* Check if it is a comment or new line character: */ if(firsttoken[0]=='#') continue; /* We are now in a data row: */ if(s0==0) /* We are on the first row of data, find s1. */ { s1=1; while( strtok(NULL, GAL_TXTARRAY_DELIMITERS) != NULL ) ++s1; } ++s0; } free(line); errno=0; if(fclose(fp)==EOF) error(EXIT_FAILURE, errno, "%s", filename); if(s0==0 && s1==0) error(EXIT_FAILURE, 0, "no table could be read in %s", filename); *outs0=s0; *outs1=s1; } static void savetolog(FILE **log, char *filename, size_t lineno, size_t s0, size_t s1, char *token) { if(*log) /* The file is already open. */ fprintf(*log, "%-10zu%-10zu%-10zu%s\n", lineno, s0, s1, token); else /* Not yet created. */ { errno=0; *log=fopen(GAL_TXTARRAY_LOG, "w"); if(*log==NULL) error(EXIT_FAILURE, errno, "%s", filename); fprintf(*log, "# Elements in %s which could not be read as a \n" "# number. They are saved as nan in the array.\n" "# The columns in the table below are:\n" "# 0: Line number in file.\n" "# 1: Row number in table (without commented or blank " "lines).\n" "# 2: Column number in table.\n" "# 3: The string that could not be converted to a number.\n" "# Note that counting starts from zero.\n", filename); fprintf(*log, "%-10zu%-10zu%-10zu%s\n", lineno-1, s0, s1, token); } } /* Macro functions: */ static double convertandsave(char *token, size_t lineno, char *filename, FILE *log, size_t ts0, size_t ts1) { double dout; char *tailptr=NULL; errno=0; dout=strtod(token, &tailptr); if(errno) error_at_line(EXIT_FAILURE, errno, "%s", lineno, token, filename); if(*tailptr!='\0') { savetolog(&log, filename, lineno, ts0, ts1, token); dout=NAN; } return dout; } static void filltable(char *filename, double *array, size_t s0, size_t s1) { FILE *fp, *log=NULL; char *line=NULL, *token; size_t len=200, lineno=0, ts0, ts1; /* Open the file: */ errno=0; fp=fopen(filename, "r"); if(fp==NULL) error(EXIT_FAILURE, errno, "%s", filename); /* Allocate some space for `line` with `len` elements so it can easily be freed later on. The value of `len` is arbitarary at this point, during the run, getline will change it along with the pointer to line. */ errno=0; line=malloc(len*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "ui.c: %zu bytes in readdefaults", len * sizeof *line); ts0=0; while( getline(&line, &len, fp) != -1 ) { ts1=0; ++lineno; /* Read the first token: */ token=strtok(line, GAL_TXTARRAY_DELIMITERS); /* If there are no non-delimters in the line (can happen if the line is a blank line in the end of the file). */ if(token==NULL) continue; /* Check if it is a comment or new line character: */ if(token[0]=='#') continue; /* Convert the first token and put it into the array: */ array[ts0*s1+ts1]=convertandsave(token, lineno, filename, log, ts0, ts1); ++ts1; /* Read the rest of the tokens in this line. We had to do the first token separately because of the nature of strtok: it can only be used recursively after one proper call, see the GNU C Library documentation for a complete explanation (this is a C standard function, but GNU C Library has a wonderful manual). */ while( (token=strtok(NULL, GAL_TXTARRAY_DELIMITERS))!=NULL ) { if(ts1>=s1) error_at_line(EXIT_FAILURE, 0, filename, lineno, "Too many columns on this line. The number of " "columns should be the same as the first row " "of the table."); array[ts0*s1+ts1]=convertandsave(token, lineno, filename, log, ts0, ts1); ++ts1; } if(ts10;++i) if(int_cols[i]>=s1) error(EXIT_FAILURE, 0, "gal_txtarray_array_to_txt: In int_cols[], " "%d is larger than the number of columns: %zu", int_cols[i], s1); for(i=0;accu_cols[i]>0;++i) if(accu_cols[i]>=s1) error(EXIT_FAILURE, 0, "gal_txtarray_array_to_txt: In accu_cols[], " "%d is larger than the number of columns: %zu", accu_cols[i], s1); for(i=0;i<3;++i) if(space[i]<=0) error(EXIT_FAILURE, 0, "gal_txtarray_array_to_txt: In space[], %d " "is smaller or equal to zero", space[i]); for(i=0;i<2;++i) if(prec[i]<0) error(EXIT_FAILURE, 0, "gal_txtarray_array_to_txt: In prec[], %d is " "smaller than zero", space[i]); /* Allocate the spaces: */ errno=0; fmt=malloc(s1 * sizeof(char *)); if(fmt==NULL) error(EXIT_FAILURE, errno, "txtarray, formatting of each " "column with %zu elements", s1); /* Prepare the formatting for each column */ gal_txtarray_printf_format(s1, fmt, int_cols, accu_cols, space, prec, forg); /* Open the output file: */ errno=0; fp=fopen(filename, "w"); if (fp==NULL) error(EXIT_FAILURE, errno, "%s", filename); /* Print the headers to file: */ if( comments[strlen(comments)-1]!='\n' ) fprintf(fp, "%s\n", comments); else fprintf(fp, "%s", comments); /* Print the data to file: */ for(i=0;i Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include "timing.h" /* Used to generate random numbers. */ unsigned long int gal_timing_time_based_rng_seed() { struct timeval tv; gettimeofday(&tv,0); return tv.tv_sec + tv.tv_usec; } /* Used to report the time it takes for an action to be done. */ void gal_timing_report(struct timeval *t1, char *jobname, size_t level) { double dt=1e30; struct timeval t2; if(level<2 && t1) { gettimeofday(&t2, NULL); dt= ( ((double)t2.tv_sec+(double)t2.tv_usec/1e6) - ((double)t1->tv_sec+(double)t1->tv_usec/1e6) ); } if(level==0) printf("%s %-f seconds\n", jobname, dt); else if(level==1) { if(t1) printf(" - %-"GAL_TIMING_VERB_MSG_LENGTH_T"s %f seconds\n", jobname, dt); else printf(" - %-"GAL_TIMING_VERB_MSG_LENGTH_T"s\n", jobname); } else if(level==2) printf(" ---- %s\n", jobname); } gnuastro-0.2.33-8a3b/lib/threads.c0000644000175000017500000001465113001632540013462 00000000000000/********************************************************************* Functions to facilitate using threads. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include /*****************************************************************/ /********* Implementation of pthread_barrier ***************/ /*****************************************************************/ /* Re-implementation of the example code given in: http://blog.albertarmea.com/post/47089939939/using-pthread-barrier-on-mac-os-x */ #if GAL_GNUASTRO_HAVE_PTHREAD_BARRIER == 0 /* Initialize the barrier structure. A barrier is a high-level way to wait until several threads have finished. */ int pthread_barrier_init(pthread_barrier_t *b, pthread_barrierattr_t *attr, unsigned int limit) { int err; /* Sanity check: */ if(limit==0) { errno = EINVAL; error(EXIT_FAILURE, errno, "in pthread_barrier_init, limit is zero"); } /* Initialize the mutex: */ err=pthread_mutex_init(&b->mutex, 0); if(err) error(EXIT_FAILURE, err, "inializing mutex in pthread_barrier_init"); /* Initialize the condition variable: */ err=pthread_cond_init(&b->cond, 0); if(err) { pthread_mutex_destroy(&b->mutex); error(EXIT_FAILURE, err, "inializing cond in pthread_barrier_init"); } /* set the values: */ b->limit=limit; b->condfinished=b->count=0; return 0; } /* Suspend the calling thread (tell it to wait), until the limiting number of barriers is reached by the other threads. When the number isn't reached yet (process goes into the `else'), then we use the `pthread_cond_wait' function, which will wait until a broadcast is announced by another thread that succeeds the `if'. After the thread no longer needs the condition variable, we increment `b->condfinished' so `pthread_barrier_destroy' can know if it should wait (sleep) or continue.*/ int pthread_barrier_wait(pthread_barrier_t *b) { pthread_mutex_lock(&b->mutex); ++b->count; if(b->count >= b->limit) { pthread_cond_broadcast(&b->cond); ++b->condfinished; pthread_mutex_unlock(&b->mutex); return 1; } else { /* Initially b->count is smaller than b->limit, otherwise control would never have reached here. However, when it get to `pthread_cond_wait', this thread goes into a suspended period and is only awaken when a broad-cast is made. But we only want this thread to finish when b->count >= b->limit, so we have this while loop. */ while(b->count < b->limit) pthread_cond_wait(&b->cond, &b->mutex); ++b->condfinished; pthread_mutex_unlock(&b->mutex); return 0; } } /* Wait until all the threads that were blocked behind this barrier have finished (don't need the mutex and condition variable anymore. Then destroy the two. After this function, you can safely re-use the pthread_barrier_t structure. */ int pthread_barrier_destroy(pthread_barrier_t *b) { struct timespec request, remaining; /* Wait until no more threads need the barrier. */ request.tv_sec=0; request.tv_nsec=GAL_THREADS_BARRIER_DESTROY_NANOSECS; while( b->condfinished < b->limit ) nanosleep(&request, &remaining); /* Destroy the condition variable and mutex */ pthread_cond_destroy(&b->cond); pthread_mutex_destroy(&b->mutex); return 0; } #endif /* GAL_GNUASTRO_HAVE_PTHREAD_BARRIER == 0 */ /*******************************************************************/ /************ Distribute job indexs in threads **************/ /*******************************************************************/ /* We have `numactions` jobs and we want their indexs to be divided between `numthreads` CPU threads. This function will give each index to a thread such that the maximum difference between the number of images for each thread is 1. The results will be saved in a 2D array of `outthrdcols` columns and each row will finish with a (size_t) -1, which is larger than any possible index!. */ void gal_threads_dist_in_threads(size_t numactions, size_t numthreads, size_t **outthrds, size_t *outthrdcols) { size_t *sp, *fp; size_t i, *thrds, thrdcols; *outthrdcols = thrdcols = numactions/numthreads+2; errno=0; thrds=*outthrds=malloc(numthreads*thrdcols*sizeof *thrds); if(thrds==NULL) error(EXIT_FAILURE, errno, "allocating thrds in prepindexsinthreads"); /* Initialize all the elements to NONINDEX. */ fp=(sp=thrds)+numthreads*thrdcols; do *sp=GAL_THREADS_NON_THRD_INDEX; while(++sp Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include "mode.h" /**************************************************************** ***************** Mininum and Maximum ******************** ****************************************************************/ /* Find the the minimum (non-blank) value in an array of type long. Note that the long type doesn't have a NaN value like the floats above. So as blank pixels, a value in the range of acceptable values is given. so we have to explicitly ignore those values.*/ void gal_statistics_long_non_blank_min(long *in, size_t size, long *min, long blank) { long tmin=INT32_MAX, *lpt; lpt=in+size; do if(*in!=blank && *intmax) tmax=*in; while(++intmax) tmax=*in; while(++intmax) tmax=*in; while(++intmax) tmax=*in; while(++intmax) tmax=*in; while(++inmax) { smax=max; max=*in; } else if(*in>smax) smax=*in; } while(++intmax) tmax=*f; if (*ftmax) tmax=*d; if (*dtmax) { tmax=*pt; tindex=pt-in; } while(++pttmax) { tmax=*pt; tindex=pt-in; } while(++ptonebinvalue) break; if(i!=numbins) { diff=onebinvalue-bins[i*2]; for(i=0;i0. You have given asked for %ld", (long)numbins); /* Fill the histogram. */ for(i=0;ibins[numbins*2]+1e-6f) break; } else while(sorted[i]>=bins[(histrow+1)*2]) if(++histrow==numbins-1) break; /* For a check: printf(" histrow: %zu\n", histrow); */ ++bins[histrow*2+1]; } /* In case a normalized histogram is desired: */ if(normhist) for(i=0;imax) max=bins[i*2+1]; for(i=0;ibins[numbins*2]+1e-6f) break; } else while(sorted[i]>=bins[(cfprow+1)*2]) { /* We have not yet reached the last bin. But we have reached the sorted[i] that is larger than the current bin and we want to switch to the next bin. So we have to finalize the current bin value. bins[cfprow*2+1] has kept the sum of all the indexs that lie within this bin. Using numinds, we also kept a count of how many indexs there was. In case there were no indexs in this bin, then we have to pass on the previous value (since this bin did not contribute any data). We set numinds=0 and start working on the next bin. */ if(numinds>0) prevind=bins[cfprow*2+1]/=numinds; /* Divide by num indexs */ else bins[cfprow*2+1]=prevind; numinds=0; if(++cfprow==numbins-1) break; } /* We can't plot every index, also in every bin, there might be a sharp gradient. So in order to make things smooth, the value given to each bin will be the average of all the indexs that like over that bin. Here we keep the sum and number of indexs so in the end we can find the average. */ bins[cfprow*2+1]+=i; ++numinds; } /* The last bin was not finalized. So we will do that here: */ bins[cfprow*2+1] = numinds>0 ? bins[cfprow*2+1]/numinds : prevind; /* For a normalized CFP: */ if(normcfp) for(i=0;i1.0f) error(EXIT_FAILURE, 0, "the quantile in gal_statistics_index_from_quantile " "(statistics.c) Should be smaller"); /* Find the index of the quantile. */ floatindex=(float)size*quant; /* printf("quant: %f, size: %zu, findex: %f\n", quant, size, floatindex); */ /* Note that in the conversion from float to size_t, the floor integer value of the float will be used. */ if( floatindex - (int)floatindex > 0.5 ) return floatindex+1; else return floatindex; } /**************************************************************** ***************** Sigma clip ******************** ****************************************************************/ /* This function will repeatedly sigma clip the data and return the median. It is assumed that the data have been ordered. o1_n0: Ordered (1), not ordered (0). */ int gal_statistics_sigma_clip_converge(float *array, int o1_n0, size_t num_elem, float sigma_multiple, float accuracy, float *outave, float *outmed, float *outstd, int print) { size_t counter=0; float *start, *oldstart, *dpt; float ave=*outave, med=*outmed, std=*outstd; float oldstd=0, oldmed=0, oldave=0, *orderedarray; if(o1_n0==0) { gal_array_float_copy(array, num_elem, &orderedarray); qsort(orderedarray, num_elem, sizeof*orderedarray, gal_qsort_float_increasing); } else orderedarray=array; start=orderedarray; while(counter0 && (oldstd-std)/stdmed-sigma_multiple*std) { start=dpt; break; } for(dpt=oldstart+num_elem-1;dpt>start;dpt--) if (*dptmed-sigma_multiple*std) { start=dpt; break; } for(dpt=oldstart+num_elem-1;dpt>start;dpt--) if (*dptmaxhist) maxhist=bins[i*2+1]; for(i=0;imsize) maxcfp=size; else maxcfp=msize; errno=0; fp=fopen(cfpsname, "w"); if(fp==NULL) error(EXIT_FAILURE, errno, "could not open file %s", cfpsname); fprintf(fp, "# Cumulative frequency plot (average index in bin) of\n" "# Actual and mirrored distributions.\n"); fprintf(fp, "# Column 0: Value in the middle of this bin.\n"); fprintf(fp, "# Column 1: Actual data.\n"); fprintf(fp, "# Column 2: Mirror distribution.\n"); for(i=0;iGAL_MODE_SYM_GOOD && modequant>GAL_MODE_LOW_QUANT_GOOD */ void gal_statistics_mode_index_in_sorted(float *sorted, size_t size, float errorstdm, size_t *modeindex, float *modesym) { struct gal_statistics_mode_params mp; /* Initialize the gal_mode_params structure: */ mp.size=size; mp.sorted=sorted; mp.tolerance=0.01; mp.numcheck=size/2; mp.errorstdm=errorstdm; if(mp.numcheck>1000) mp.interval=mp.numcheck/1000; else mp.interval=1; mp.lowi = gal_statistics_index_from_quantile(size, GAL_STATISTICS_MODE_LOW_QUANTILE); mp.highi = gal_statistics_index_from_quantile(size, GAL_STATISTICS_MODE_HIGH_QUANTILE); mp.midi = (((float)mp.highi + MODE_GOLDEN_RATIO*(float)mp.lowi) /(1+MODE_GOLDEN_RATIO)); mp.midd = mirrormaxdiff(mp.sorted, mp.size, mp.midi, mp.numcheck, mp.interval, mp.errorstdm); /* Do the golden section search and find the resulting symmetricity. */ *modeindex=modegoldenselection(&mp); modesymmetricity(sorted, size, *modeindex, errorstdm, modesym); } gnuastro-0.2.33-8a3b/lib/spatialconvolve.c0000644000175000017500000001566113001632540015243 00000000000000/********************************************************************* SpatialConvolve - Convolve an image in the spatial domain. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include /*******************************************************************/ /************** Each thread ****************/ /*******************************************************************/ void gal_spatialconvolve_pparams(float *input, size_t is0, size_t is1, float *kernel, size_t ks0, size_t ks1, size_t nt, int edgecorrection, float *out, size_t *indexs, struct gal_spatialconvolve_params *scp) { /* Put the simple values in: */ scp->is0=is0; scp->is1=is1; scp->ks0=ks0; scp->ks1=ks1; scp->out=out; scp->input=input; scp->kernel=kernel; scp->indexs=indexs; scp->numthreads=nt; scp->edgecorrection=edgecorrection; } void * gal_spatialconvolve_thread(void *inparam) { struct gal_spatialconvolve_params *scp= (struct gal_spatialconvolve_params *)inparam; double sum, ksum; long naxes[2]={scp->is1, scp->is0}; float *f, *fp, *k, *istart, *kstart; int edgecorrection=scp->edgecorrection; size_t is1=scp->is1, ks0=scp->ks0, ks1=scp->ks1; long *fpixel_i=scp->fpixel_i, *lpixel_i=scp->lpixel_i; long *fpixel_o=scp->fpixel_o, *lpixel_o=scp->lpixel_o; size_t i, j, ind, *indexs=scp->indexs, numrows, numcols; float *input=scp->input, *kernel=scp->kernel, *out=scp->out; /* Go over all the pixels associated with this thread. */ for(i=0;indexs[i]!=GAL_THREADS_NON_THRD_INDEX;++i) { /* Set the index, if it is a NaN pixel, then set the output to be NaN too. */ ind=indexs[i]; if(isnan(input[ind])) { out[ind]=NAN; continue; } /* Set the starting and ending pixels on the kernel, note that the overlap function in box.c uses FITS coordinates. */ fpixel_o[0]=1; fpixel_o[1]=1; lpixel_o[0]=ks1; lpixel_o[1]=ks0; fpixel_i[0]=ind%is1+1-ks1/2; fpixel_i[1]=ind/is1+1-ks0/2; lpixel_i[0]=ind%is1+1+ks1/2; lpixel_i[1]=ind/is1+1+ks0/2; gal_box_overlap(naxes, fpixel_i, lpixel_i, fpixel_o, lpixel_o); /* fpixels and lpixels now point to the overlap's starting and ending both on the image and on the kernel. */ sum=0.0f; numcols=lpixel_i[0]-fpixel_i[0]+1; /* lpixel is inside the box. */ numrows=lpixel_i[1]-fpixel_i[1]+1; /* lpixel is inside the box. */ ksum = edgecorrection ? 0.0f : 1.0f; istart = &input[ (fpixel_i[1]-1) * is1 + fpixel_i[0]-1 ]; kstart = &kernel[ (fpixel_o[1]-1) * ks1 + fpixel_o[0]-1 ]; for(j=0;jnumthreads>1) pthread_barrier_wait(scp->b); return NULL; } /*******************************************************************/ /************** Outside function ****************/ /*******************************************************************/ void gal_spatialconvolve_convolve(float *input, size_t is0, size_t is1, float *kernel, size_t ks0, size_t ks1, size_t numthreads, int edgecorrection, float **out) { int err; pthread_t t; /* All thread ids saved in this, not used. */ pthread_attr_t attr; pthread_barrier_t b; struct gal_spatialconvolve_params *scp; size_t i, nb, *indexs, thrdcols; /* Array keeping thread parameters for each thread. */ errno=0; scp=malloc(numthreads*sizeof *scp); if(scp==NULL) error(EXIT_FAILURE, errno, "%zu bytes in gal_spatialconvolve_convolve " "(spatialconvolve.c) for scp", numthreads*sizeof *scp); /* Allocate the output array: */ errno=0; *out=malloc(is0*is1*sizeof **out); if(*out==NULL) error(EXIT_FAILURE, errno, "%zu bytes for convolution output", is0*is1*sizeof **out); /* Distribute the image pixels into the threads: */ gal_threads_dist_in_threads(is0*is1, numthreads, &indexs, &thrdcols); /* Start the convolution. */ if(numthreads==1) { gal_spatialconvolve_pparams(input, is0, is1, kernel, ks0, ks1, numthreads, edgecorrection, *out, indexs, &scp[0]); gal_spatialconvolve_thread(&scp[0]); } else { /* Initialize the attributes. Note that this running thread (that spinns off the numthreads threads) is also a thread, so the number the barrier should be one more than the number of threads spinned off. */ if(is0*is1 Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include /* Initialize the array for sorting indexs to NULL. */ float *gal_qsort_index_arr; int gal_qsort_index_float_decreasing(const void * a, const void * b) { float ta=gal_qsort_index_arr[ *(size_t *)a ]; float tb=gal_qsort_index_arr[ *(size_t *)b ]; return (tb > ta) - (tb < ta); } int gal_qsort_int_decreasing(const void * a, const void * b) { return ( *(int*)b - *(int*)a ); } int gal_qsort_int_increasing(const void * a, const void * b) { return ( *(int*)a - *(int*)b ); } int gal_qsort_float_decreasing(const void * a, const void * b) { float ta=*(float*)a; float tb=*(float*)b; return (tb > ta) - (tb < ta); } int gal_qsort_float_increasing(const void * a, const void * b) { float ta=*(float*)a; float tb=*(float*)b; return (ta > tb) - (ta < tb); } int gal_qsort_double_decreasing(const void * a, const void * b) { double ta=*(double*)a; double tb=*(double*)b; return (tb > ta) - (tb < ta); } int gal_qsort_double_increasing(const void * a, const void * b) { double ta=*(double*)a; double tb=*(double*)b; return (ta > tb) - (ta < tb); } gnuastro-0.2.33-8a3b/lib/polygon.c0000644000175000017500000003345413001632540013521 00000000000000/********************************************************************* Polygon related functions and macros. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /***************************************************************/ /************** MACROS ******************/ /***************************************************************/ /* The cross product of two points from the center. */ #define GAL_POLYGON_CROSS_PRODUCT(A, B) ( (A)[0]*(B)[1] - (B)[0]*(A)[1] ) /* Find the cross product (2*area) between three points. Each point is assumed to be a pointer that has atleast two values within it. */ #define GAL_POLYGON_TRI_CROSS_PRODUCT(A, B, C) \ ( ( (B)[0]-(A)[0] ) * ( (C)[1]-(A)[1] ) - \ ( (C)[0]-(A)[0] ) * ( (B)[1]-(A)[1] ) ) \ /* We have the line A-B. We want to see if C is to the left of this line or to its right. This function will return 1 if it is to the left. It uses the basic property of vector multiplication: If the three points are anti-clockwise (the point is to the left), then the vector multiplication is positive, if it is negative, then it is clockwise (c is to the right). Ofcourse it is very important that A be below or equal to B in both the X and Y directions. The rounding error might give -0.0000000000001 (I didn't count the number of zeros!!) instead of zero for the area. Zero would indicate that they are on the same line in this case this should give a true result. */ #define GAL_POLYGON_LEFT_OF_LINE(A, B, C) \ ( GAL_POLYGON_TRI_CROSS_PRODUCT((A), (B), (C)) > -GAL_POLYGON_ROUND_ERR ) /* >= 0 */ /* See if the three points are collinear, similar to GAL_POLYGON_LEFT_OF_LINE except that the result has to be exactly zero. */ #define GAL_POLYGON_COLLINEAR_WITH_LINE(A, B, C) \ (GAL_POLYGON_TRI_CROSS_PRODUCT((A), (B), (C)) > -GAL_POLYGON_ROUND_ERR \ && GAL_POLYGON_TRI_CROSS_PRODUCT((A), (B), (C)) < GAL_POLYGON_ROUND_ERR) /* == 0 */ /* Similar to GAL_POLYGON_LEFT_OF_LINE except that if they are on the same line, this will return 0 (so that it is not on the left). Therefore the name is "proper left". */ #define GAL_POLYGON_PROP_LEFT_OF_LINE(A, B, C) \ ( GAL_POLYGON_TRI_CROSS_PRODUCT((A), (B), (C)) > GAL_POLYGON_ROUND_ERR ) /* > 0 */ #define GAL_POLYGON_MIN_OF_TWO(A, B) ((A)<(B)+GAL_POLYGON_ROUND_ERR ? (A) : (B)) #define GAL_POLYGON_MAX_OF_TWO(A, B) ((A)>(B)-GAL_POLYGON_ROUND_ERR ? (A) : (B)) /***************************************************************/ /************** Basic operations ******************/ /***************************************************************/ /* Sort the pixels in anti clock-wise order.*/ void gal_polygon_ordered_corners(double *in, size_t n, size_t *ordinds) { double angles[GAL_POLYGON_MAX_CORNERS]; size_t i, tmp, aindexs[GAL_POLYGON_MAX_CORNERS], tindexs[GAL_POLYGON_MAX_CORNERS]; if(n>GAL_POLYGON_MAX_CORNERS) error(EXIT_FAILURE, 0, "most probably a bug! The number of corners " "given to `gal_polygon_ordered_corners' is more than %d. This is an " "internal value and cannot be set from the outside. Most probably " "Some bug has caused this un-normal value. Please contact us at " PACKAGE_BUGREPORT" so we can solve this problem", GAL_POLYGON_MAX_CORNERS); /* For a check: printf("\n\nBefore sorting:\n"); for(i=0;i in[ ordinds[1]*2 ]) { tmp=ordinds[0]; ordinds[0]=ordinds[1]; ordinds[1]=tmp; } /* We only have `n-1' more elements to sort, use the angle of the line between the three remaining points and the first point. */ for(i=0;i=GAL_POLYGON_MIN_OF_TWO(Aa[0], Ab[0])-GAL_POLYGON_ROUND_ERR && o[0]<=GAL_POLYGON_MAX_OF_TWO(Aa[0], Ab[0])+GAL_POLYGON_ROUND_ERR && o[1]>=GAL_POLYGON_MIN_OF_TWO(Aa[1], Ab[1])-GAL_POLYGON_ROUND_ERR && o[1]<=GAL_POLYGON_MAX_OF_TWO(Aa[1], Ab[1])+GAL_POLYGON_ROUND_ERR ) return 1; else return 0; } else return 0; } /* Clip (find the overlap of) two polygons. This function uses the Sutherland-Hodgman polygon clipping psudocode from Wikipedia: List outputList = subjectPolygon; for (Edge clipEdge in clipPolygon) do List inputList = outputList; outputList.clear(); Point S = inputList.last; for (Point E in inputList) do if (E inside clipEdge) then if (S not inside clipEdge) then outputList.add(ComputeIntersection(S,E,clipEdge)); end if outputList.add(E); else if (S inside clipEdge) then outputList.add(ComputeIntersection(S,E,clipEdge)); end if S = E; done done The difference is that we are not using lists, but arrays to keep polygon vertices. The two polygons are called Subject (`s') and Clip (`c') with `n' and `m' vertices respectively. The output is stored in `o' and the number of elements in the output are stored in what `*numcrn' (for number of corners) points to.*/ void gal_polygon_clip(double *s, size_t n, double *c, size_t m, double *o, size_t *numcrn) { double in[2*GAL_POLYGON_MAX_CORNERS], *S, *E; size_t t, ii=m-1, i=0, jj, j, outnum, innum; /* if(n>GAL_POLYGON_MAX_CORNERS || m>GAL_POLYGON_MAX_CORNERS) error(EXIT_FAILURE, 0, "the two polygons given to the function " "gal_polygon_clip in polygon.c have %zu and %zu vertices. They cannot" " have any values larger than %zu", n, m, GAL_POLYGON_MAX_CORNERS); */ /* 2*outnum because for each vertice, there are two elements. */ outnum=n; for(t=0;t<2*outnum;++t) o[t]=s[t]; while(i0) ++outnum; o[2*outnum]=E[0]; o[2*outnum+1]=E[1]; ++outnum; } else if( GAL_POLYGON_PROP_LEFT_OF_LINE(&c[ii*2], &c[i*2], S) ) if( seginfintersection(S, E, &c[ii*2], &c[i*2], &o[2*outnum])>0 ) ++outnum; /* { size_t k; printf("(%.3f, %.3f) -- (%.3f, %.3f): %zu\n", S[0], S[1], E[0], E[1], outnum); for(k=0;k Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include "mode.h" /**************************************************************** ***************** Mode plots ******************** ****************************************************************/ /* This is the python code you can put in `plot.py` so the plot command mentioned here works: ----------------------------------------------------------------- #! /usr/bin/env python3 import sys import numpy as np import matplotlib.pyplot as plt a=np.loadtxt(sys.argv[1]) b=np.loadtxt(sys.argv[2]) w=a[1,0]-a[0,0] plt.bar(a[:,0], a[:,1], width=w, color="blue", linewidth=0, alpha=0.6) plt.bar(a[:,0], a[:,2], width=w, color="green", linewidth=0, alpha=0.4) plt.plot(b[:,0], b[:,1], linewidth=2, color="blue") plt.plot(b[:,0], b[:,2], linewidth=2, color="green") plt.ylim([0,np.amax(a[:,1])]) plt.xlim([np.amin(a[:,0]),np.amax(a[:,0])]) plt.savefig(sys.argv[3]) --------------------------------------------------------- Run it with `./plot.py histsname.txt cfpsname.txt outputpdfname.pdf` It will plot the corresponding histograms and cumulative frequency plots. If you like to, this call is available as a system() call in the functions below. */ /* This is used for the plots, it will allocate an array and put the mirrored array values in it. `mi` is the index the mirror is to be placed on. */ void makemirrored(float *in, size_t mi, float **outmirror, size_t *outsize) { size_t i, size; float *mirror, zf; zf=in[mi]; size=2*mi+1; errno=0; mirror=malloc(size*sizeof *mirror); if(mirror==NULL) error(EXIT_FAILURE, errno, "%zu bytes for mirror array in " "makemirrored (mode.c)", size*sizeof *mirror); for(i=0;i<=mi;++i) mirror[i] = in[i]; for(i=1;i<=mi;++i) mirror[mi+i] = 2*zf - mirror[mi-i]; *outmirror=mirror; *outsize=size; } /**************************************************************** ***************** Mode ******************** ****************************************************************/ /*Find the index where the two CDFs dirverge beyond CDFSDIVERGEDIFF. T he input CDF and a CDF of a mirrored distribution about the quantile `mirrorquant` are compared. The basic idea behind finding the mode is comparing the mirrored CDF (about a test for the mode) with the actual CDF for a given point. This is the job of this function. It takes the ordered array and the quantile that is to be checked, it then finds the maximum difference between the mirrored CDF about the given point and the input CDF. `zf` keeps the flux at the mirror (zero) point. `i` is used to count the pixels before m. So `m+i` is the index of the mirrored distribution and mf=zf+(zf-a[m-i])=2*zf-a[m-i] is the mirrored flux at this point. `j` is found such that a[m+j] has the nearest flux to `mf`. The desired difference between the input CDF and the mirrored one for each `i` is then simply: `j-i`. Once `i` is incremented, `mf` will increase, so to find the new `j` we don't need to begin looking from `j=0`. Remember that the array is sorted, so the desired `j` is definitely larger than the previous `j`. So, if we keep the previous `j` in `prevj` then, all we have to do is to start incrementing `j` from `prevj`. This will really help in speeding up the job :-D. Only for the first element, `prevj=0`.*/ size_t mirrormaxdiff(float *a, size_t size, size_t m, size_t numcheck, size_t interval, size_t stdm) { /* The variables: i: Index on mirror distribution. j: Index on input distribution. prevj: Index of previously checked point in the actual array. mf: Flux that is approximately equal in both distributions.*/ float mf, zf; size_t maxdiff=0, errordiff; size_t i, j, absdiff, prevj=0; /* Find the error and mirror flux value */ zf=a[m]; errordiff=stdm*sqrt(m); /* printf("###############\n###############\n"); printf("### Mirror pixel: %zu\n", m); printf("###############\n###############\n"); */ /* Go over the mirrored points. */ for(i=1; imf, we have reached the last pixel to check. Now we just have to see if a[m+j-1] is closer to mf or if a[m+j]. We change `j` accordingly and break out of the `j` loop. */ for(j=prevj;jmf) { if( a[m+j]-mf < mf-a[m+j-1] ) break; else { j--; break; } } /* printf("i:%-5zu j:%-5zu diff:%-5d maxdiff: %zu\n", i, j, (int)j-(int)i, maxdiff); */ /* The index of the actual CDF corresponding the the mirrored flux has been found. We want the mirrored distribution to be within the actual distribution, not beyond it, so the only acceptable results are when ij+errordiff then the result is not acceptable! */ if(i>j+errordiff) { maxdiff = MODE_MIRROR_IS_ABOVE_RESULT; break; } absdiff = i>j ? i-j : j-i; if(absdiff>maxdiff) maxdiff=absdiff; prevj=j; } return maxdiff; } /* Find the mode of a float array of size `size`. I assume that mirrormaxdiff() has one minimum (within the statistical errors) in the function. To find that minimum, the golden section search algorithm is going to used. Read the Wikipedia article for a very nice introduction. In summary we will constantly be finding middle points in the given interval and thus decreasing the interval until a certain tolerance is reached. If the input interval is on points `a` and `b`, then the middle point (lets call it `c`, where c>a and chighi-mp->midi > mp->midi-mp->lowi) di = mp->midi + MODE_TWO_TAKE_GOLDEN_RATIO *(float)(mp->highi-mp->midi); else di = mp->midi - MODE_TWO_TAKE_GOLDEN_RATIO * (float)(mp->midi-mp->lowi); /* Since these are all indexs (and positive) we don't need an absolute value, highi is also always larger than lowi! In some cases, the first (standard) condition might be satisfied, while highi-lowi<=2. In such cases, also jump out! */ if( (mp->highi - mp->lowi) < mp->tolerance*(mp->midi+di) || (mp->highi - mp->lowi) <= 3) return (mp->highi+mp->lowi)/2; /* Find the maximum difference for this quantile. */ dd = mirrormaxdiff(mp->sorted, mp->size, di, mp->numcheck, mp->interval, mp->errorstdm); /*------------------------------------------------------------------ sprintf(outname, "%dcmp.pdf", counter); sprintf(cfpsname, "%dcfps.txt", counter); sprintf(histsname, "%dhists.txt", counter); gal_mode_make_mirror_plots(mp->sorted, mp->size, di, histsname, cfpsname); sprintf(command, "./plot.py %s %s %s", histsname, cfpsname, outname); system(command); -------------------------------------------------------------------*/ /* printf("%-5zu\t%-5zu(%d)\t%-5zu ----> dq: %-5zu di: %d\n", mp->lowi, mp->midi, (int)mp->midd, mp->highi, di, (int)dd); */ /* +++++++++++++ The mirrored distribution's cumulative frequency plot has be lower than the actual's cfp. If it isn't, `di` will be GAL_MODE_MIRROR_IS_ABOVE_RESULT. In this case, the normal golden section minimization is not going to give us what we want. So I have added this modification to it. In such cases, we want the search to go to the lower intervals.*/ if(dd==MODE_MIRROR_IS_ABOVE_RESULT) { if(mp->midi < di) { mp->highi=di; return modegoldenselection(mp); } else { mp->highi=mp->midi; mp->midi=di; mp->midd=dd; return modegoldenselection(mp); } } /* +++++++++++++ End of my addition to the golden section search. */ /* This is the standard golden section search: */ if(ddmidd) { if(mp->highi-mp->midi > mp->midi-mp->lowi) { mp->lowi = mp->midi; mp->midi = di; mp->midd = dd; return modegoldenselection(mp); } else { mp->highi = mp->midi; mp->midi = di; mp->midd = dd; return modegoldenselection(mp); } } else { if(mp->highi-mp->midi > mp->midi-mp->lowi) { mp->highi = di; return modegoldenselection(mp); } else { mp->lowi = di; return modegoldenselection(mp); } } } /* Once the mode is found, we need to do a quality control. This quality control is the measure of symmetricity. Lets assume the mode index is at `m`, the error in `m` can be assumed to be sqrt(m). So lets call the first point that the difference between the cumulative distribution of the mirror and actual data deviate above sqrt(m), is at index `b`. For a scale parameter, lets assume that the index of 5% of `m` is `a`. We could have taken the distribution minimum, but the scatter in that can be too high! Now the symmetricity of the mode can be quantified as: (b-m)/(m-a). For a completly symmetric mode, this should be 1. Note that the search for `b` only goes to the 95% of the distribution. */ void modesymmetricity(float *a, size_t size, size_t mi, float errorstdm, float *sym) { float af, bf, mf, fi; size_t i, j, bi=0, topi, errdiff, prevj=0; mf=a[mi]; errdiff=errorstdm*sqrt(mi); topi = 2*mi>size-1 ? size-1 : 2*mi; af=a[gal_statistics_index_from_quantile(2*mi+1, GAL_STATISTICS_MODE_SYMMETRICITY_LOW_QUANT)]; /* This loop is very similar to that of mirrormaxdiff(). It will find the index where the difference between the two cumulative frequency plots exceeds that of the error in the mirror index. */ for(i=1; ifi) { if( a[mi+j]-fi < fi-a[mi+j-1] ) break; else { j--; break; } } if(i>j+errdiff || j>i+errdiff) { bi=mi+i; break; } prevj=j; } /* bi==0 shows that no point with a larger difference could be found. So bi should be set to the end of the search region. */ if(bi==0) bi=topi; bf=a[bi]; /* printf("%f, %f, %f\n", af, mf, bf); */ *sym=(bf-mf)/(mf-af); /* This is mainly used for plotting, which subtracts `mf`. printf("SymmetricFlux: %f\n", a[bi]-mf); printf("symmetricity: %f\n", sym); */ } gnuastro-0.2.33-8a3b/lib/mesh.c0000644000175000017500000017260313001632540012766 00000000000000/********************************************************************* meshgrid -- Create a mesh grid ready for multithreaded analysis. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include "neighbors.h" /* Basic idea ========== The meshes in an image are completely independent. There is no overlap. So when we want to do any sort of processing on separate meshes, they can be done completely independently. Whether they are positioned in the same channel or not. Usually, after the initial processing is complete, and some meshes pass the test and some don't, we need to do interpolation to find values for all the meshes and finally smooth the result. The programs outside of mesh.c, should only be using garray (1 or 2). Not cgarray or fgarray. The reason for this is that the user might choose to ignore channels on one step and use them in another. All the functions in mesh.c will set garray and use cgarray and fgarray such that when they return, garray points to their output. So the caller to any of these functions doesn't have to worry about which one was last used, they can just ignorantly use garray and everything will be fine. Maybe in the future all these arrays can be removed and calculated immediately for each mesh during the processing. This might increase the speed and decrease the amount of necessary memory. However, it will add to the complexity of the code. So at this early stage, I am doing this job separately here for now so the main functions can be cleaner and more easily understandable. Once they have become mature enough, all these calculations should be done during the processing of each mesh. */ /*********************************************************************/ /************ Finding the proper mesh ID ******************/ /*********************************************************************/ /* This is useful for when you are going over the elements in garray (and you are completley ignorant to which one of cgarrays or fgarrays garray points to) and you need the channel based IDs to get basic mesh information like the mesh type and size. */ size_t gal_mesh_ch_based_id_from_gid(struct gal_mesh_params *mp, size_t gid) { if(mp->nch==1 || mp->garray1==mp->cgarray1) return gid; else { /* The X and Y of this mesh in the full image: */ size_t f0=gid/(mp->gs1*mp->nch1), f1=gid%(mp->gs1*mp->nch1); /* The channel ID: */ size_t chid = (f0/mp->gs0) * mp->nch1 + f1/mp->gs1; /* The ID of this mesh in this channel: */ size_t inchannelid = (f0%mp->gs0) * mp->gs1 + f1%mp->gs1; /* For a check: printf("%zu:\n\t(f0, f1): (%zu, %zu)\t chid: %zu\tinchannelid: %zu\n", gid, f0, f1, chid, inchannelid); */ /* Return the channel-based ID: */ return chid * mp->nmeshc + inchannelid; } /* This function should not reach here! If it does there is problem, so just return an impossible value so the root of the issue can be found easily: */ return (size_t)(-1); } /* Get the garray-based ID from the channel-based ID. See the comments above gal_mesh_ch_based_id_from_gid for a complete explanation. */ size_t gal_mesh_gid_from_ch_based_id(struct gal_mesh_params *mp, size_t chbasedid) { if(mp->nch==1 || mp->garray1==mp->cgarray1) return chbasedid; else { /* The X and Y positions of this channel in the channels array: */ size_t chx=(chbasedid/mp->nmeshc)/mp->nch1; size_t chy=(chbasedid/mp->nmeshc)%mp->nch1; /* The X and Y of this mesh in this channel: */ size_t mx=(chbasedid%mp->nmeshc)/mp->gs1; size_t my=(chbasedid%mp->nmeshc)%mp->gs1; /* For a check: printf("%zu:\n\t(chx, chy): (%zu, %zu)" "\n\t(mx, my): (%zu, %zu)" "\n\t%zu\n\n", chbasedid, chx, chy, mx, my, (chx*mp->gs0+mx) * mp->nch1 + (chy*mp->gs1+my)); */ /* Return the : */ return (chx*mp->gs0+mx) * mp->nch1 + (chy*mp->gs1+my); } /* This function should not reach here! If it does there is problem, so just return an impossible value so the root of the issue can be found easily: */ return (size_t)(-1); } /* The user has a pixel index in the final image and wants to know the id it should plug into the garrays to get a value for this pixel. This is the job of this function. So to find the value on the mesh grid for a pixel at index `ind', the user should just run: mp->garray[imgindextomeshid(mp, ind)] */ size_t gal_mesh_img_xy_to_mesh_id(struct gal_mesh_params *mp, size_t x, size_t y) { /* Take the proper action. The ternary conditional is here because when the meshsize is not an exact multiple of the the channel (image) size, there might be some extra pixels in the last mesh in each dimension which will cause trouble in the end. So without these checks, a pixel lying in those extra regions will be thought of as belongin to another mesh (that doesn't exist). We have to make sure that doesn't happen. */ if(mp->nch==1) return ( (x/mp->meshsizegs0 ? x/mp->meshsize : x/mp->meshsize -1) * mp->gs1 + (y/mp->meshsizegs1 ? y/mp->meshsize : y/mp->meshsize -1)); else { /* Number of pixels along each axis in all channels: */ size_t cps0=mp->s0/mp->nch2, cps1=mp->s1/mp->nch1; /* The X and Y positions of this channel in the channels array: */ size_t chx=x/cps0, chy=y/cps1; /* The X and Y of this mesh in this channel: */ size_t mx = (x%cps0)/mp->meshsize; size_t my = (y%cps1)/mp->meshsize; /* If the last mesh doesn't have the same size as the rest, mx or my might become one larger. Note that we have already made sure that this pixel is in the channel specified by chx and chy. */ mx = mxgs0 ? mx : mx-1; my = mygs1 ? my : my-1; /* Return the proper id to input into garray. */ if(mp->garray1==mp->cgarray1) return mp->nmeshc * (chx*mp->nch1+chy) + mx * mp->gs1 + my; else return (chx*mp->gs0+mx) * mp->gs1 + (chy * mp->gs1 + my); } /* This function should not reach here! So we will just return a value that will always be problematic ;-). */ return (size_t) -1; } /*********************************************************************/ /******************** Full garray ********************/ /*********************************************************************/ /* By default, the garray1 and garray2 arrays keep the meshes of each channel contiguously. So in practice, each channel is like a small independent image. This will cause problems when we want to work on the meshs irrespective of which channel they belong to. This function allocates and fills in the fgarray1 and fgarray2 arrays. The explanation above is for the case when reverse==0. If it is set equal to 1 (or any non-zero number), then */ void gal_mesh_full_garray(struct gal_mesh_params *mp, int reverse) { size_t nch1=mp->nch1; size_t ind, gs1=mp->gs1, gs0=mp->gs0; float *fgarray1=NULL, *fgarray2=NULL; float *cgarray1=mp->cgarray1, *cgarray2=mp->cgarray2; size_t g0, g1, f0, f1, fmeshind, chid, is1=mp->nch1*mp->gs1; /* First allocate the fgarrays if they were not already allocated. */ if(mp->fgarray1==NULL) { /* A simple sanity check */ if(reverse) error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we can " "fix this problem. For some reason, gal_mesh_full_garray " "has been called with the `reverse' flag set to true while " "fgarray is not allocated! This should not happen", PACKAGE_BUGREPORT); /* Allocate the fgarrays */ errno=0; mp->fgarray1=malloc(mp->nmeshi*sizeof *mp->fgarray1); if(mp->fgarray1==NULL) error(EXIT_FAILURE, errno, "%zu bytes for mp->fgarray1 (mesh.c)", mp->nmeshi*sizeof *mp->fgarray1); } if(mp->ngarrays==2 && mp->fgarray2==NULL) { errno=0; mp->fgarray2=malloc(mp->nmeshi*sizeof *mp->fgarray2); if(mp->fgarray2==NULL) error(EXIT_FAILURE, errno, "%zu bytes for mp->fgarray2 (mesh.c)", mp->nmeshi*sizeof *mp->fgarray2); } fgarray1=mp->fgarray1; fgarray2=mp->fgarray2; /* Fill the fgarrays or cgarrays with the proper values: */ for(chid=0;chidnch;++chid) { /* The first pixel ID in this channel is: chid*mp->nmeshi. */ f0=(chid/nch1)*gs0; /* Position of first channel mesh */ f1=(chid%nch1)*gs1; /* in full image. */ fmeshind=chid*mp->nmeshc; /* Go over all the meshes in this channel and put them in their righful place. */ for(ind=0;indnmeshc;++ind) { g0=ind/gs1; /* Position of this mesh in this channel. */ g1=ind%gs1; if(reverse) cgarray1[ind+fmeshind]=fgarray1[(g0+f0)*is1+g1+f1]; else fgarray1[(g0+f0)*is1+g1+f1]=cgarray1[ind+fmeshind]; if(mp->ngarrays==2) { if(reverse) cgarray2[ind+fmeshind]=fgarray2[(g0+f0)*is1+g1+f1]; else fgarray2[(g0+f0)*is1+g1+f1]=cgarray2[ind+fmeshind]; } } } /* Just for a check: gal_fits_array_to_file("nochannels.fits", "fgarray1", FLOAT_IMG, fgarray1, mp->nch2*mp->gs0, mp->nch1*mp->gs1, 1, NULL, NULL, "mesh"); if(mp->ngarrays==2) gal_fits_array_to_file("nochannels.fits", "fgarray2", FLOAT_IMG, fgarray2, mp->nch2*mp->gs0, mp->nch1*mp->gs1, 1, NULL, NULL, "mesh"); */ } /*********************************************************************/ /******************** Checking functions ********************/ /*********************************************************************/ /* Save the meshid of each pixel into an array the size of the image. */ void gal_mesh_check_mesh_id(struct gal_mesh_params *mp, long **out) { long i, *l, *lp; size_t row, start, *types=mp->types; size_t s0, s1, is1=mp->s1, *ts0=mp->ts0, *ts1=mp->ts1; /* Allocate the array to keep the mesh indexs. Calloc is used so we can add all the indexes to the existing value to make sure that there is no overlap. */ errno=0; *out=calloc(mp->s0*mp->s1, sizeof **out); if(*out==NULL) error(EXIT_FAILURE, errno, "the array to show mesh labels in checkmesh"); /* Fill the indexs: */ for(i=0;inmeshi;++i) { row=0; s0=ts0[types[i]]; s1=ts1[types[i]]; start=mp->start[i]; do { lp=(l = *out + start + row++ * is1 ) + s1; do *l++ += i; while(lngarrays; size_t gid, row, start, chbasedid, *types=mp->types; size_t s0, s1, is1=mp->s1, *ts0=mp->ts0, *ts1=mp->ts1; float *f, *fp, *ff=NULL, garray1=FLT_MAX, garray2=FLT_MAX; /* Allocate the array to keep the mesh indexs. Calloc is used so we can add all the indexes to the existing value to make sure that there is no overlap. */ errno=0; *out1=malloc(mp->s0*mp->s1*sizeof **out1); if(*out1==NULL) error(EXIT_FAILURE, errno, "%zu bytes for out1 in gal_mesh_check_garray (mesh.c)", mp->s0*mp->s1*sizeof **out1); if(ngarrays==2) { errno=0; *out2=malloc(mp->s0*mp->s1*sizeof **out2); if(*out2==NULL) error(EXIT_FAILURE, errno, "%zu bytes for out2 in gal_mesh_check_garray (mesh.c)", mp->s0*mp->s1*sizeof **out2); } /* Fill the array: */ for(gid=0;gidnmeshi;++gid) { /* Set the proper meshid depending on what garray points to, see the explanation above setmeshid. */ chbasedid = gal_mesh_ch_based_id_from_gid(mp, gid); /* Fill the output array with the value in this mesh. It is really important that `i' should be used for the garrays, not cmeshid. cmeshid is only for the basic mesh parameters that it is used for. */ row=0; s0=ts0[types[chbasedid]]; s1=ts1[types[chbasedid]]; start=mp->start[chbasedid]; garray1 = mp->garray1[gid]; if(ngarrays==2) garray2 = mp->garray2[gid]; do { fp= ( f = *out1 + start + row * is1 ) + s1; if(ngarrays==2) ff= *out2 + start + row * is1; do { *f++ = garray1; if(ngarrays==2) *ff++ = garray2; } while(fmeshbasedcheck) { /* We want one pixel per mesh. If the last operation was on cgarray, then first the fgarray has to be filled. Note that when more than one channel is present, only fgarray can be used for this job. In cgarray the meshs are ordered differently. */ if(mp->garray1==mp->cgarray1) gal_mesh_full_garray(mp, 0); gal_fits_array_to_file(filename, extname1, FLOAT_IMG, mp->fgarray1, mp->gs0*mp->nch2, mp->gs1*mp->nch1, 0, wcs, NULL, spack_string); if(mp->ngarrays==2) /* Note that gal_mesh_full_garray will correct both the meshs if there are two.*/ gal_fits_array_to_file(filename, extname2, FLOAT_IMG, mp->fgarray2, mp->gs0*mp->nch2, mp->gs1*mp->nch1, 0, wcs, NULL, spack_string); } else { gal_mesh_check_garray(mp, &tmp1, &tmp2); gal_fits_array_to_file(filename, extname1, FLOAT_IMG, tmp1, mp->s0, mp->s1, 0, wcs, NULL, spack_string); if(mp->ngarrays==2) gal_fits_array_to_file(filename, extname2, FLOAT_IMG, tmp2, mp->s0, mp->s1, 0, wcs, NULL, spack_string); free(tmp1); free(tmp2); } } /*********************************************************************/ /******************** Creating the mesh ********************/ /*********************************************************************/ /* In each channel we can have four types (sizes of meshs): 0. If meshsize is chosen nicely in relation to the channel size, the majority (or ideally all) of the mesh tiles are going to have an area of meshsize*meshsize. These are built from pixel (0,0) until ((s0/mesh_size)*mesh_size, (s1/mesh_size)*mesh_size), note that these are integer divisions, not floating point, so 5/2=2. 1. The top row of meshes. If s0%meshsize is larger than a certain fraction of meshsize, they will have s0%meshsize pixels in each row. If not, they will have meshsize+s0%meshsize rows. In any case, all but the last (type 3) will have meshsize columns. The number of columns of the last mesh in the top row, will depend on the third type of meshes. 2. Just like type 2, but for the width or the number of columns in the image. 3. The size of the last (top left) mesh in the grid will get its height (number of rows) from type 2s and its width from type 3s. Note that the numbers for the types used here are only for when all four types exist, when there is only one or two types, the first (in the order above) gets type id of zero and the second gets type id of 1. In the actual function, the indexs are given in the order the types are found. */ static void fillmeshinfo(struct gal_mesh_params *mp, size_t chs0, size_t chs1, size_t lasts0, size_t lasts1) { size_t i, j, chi, chj, gs0=mp->gs0, gs1=mp->gs1; size_t meshsize=mp->meshsize, *chindex=mp->chindex; size_t numtypes=0, totalmeshcount=0, chid, s1=mp->s1; size_t meshid, typeind, lasti, lastj, nmeshc=mp->nmeshc; size_t nch1=mp->nch1, nch2=mp->nch2, *ts0=mp->ts0, *ts1=mp->ts1; size_t *types=mp->types, *start=mp->start, *imgindex=mp->imgindex; /* Initialize the maximum number of rows and columns: */ mp->maxs1=mp->maxs0=0; /* Main meshs (type 0) in each channel. If we have more than one row or column of meshes in each channel, then we will have some type1 meshes.*/ if(gs0>1 || gs1>1) { typeind=numtypes++; ts1[typeind]=ts0[typeind]=meshsize; lasti = lasts0==meshsize ? gs0 : gs0-1; lastj = lasts1==meshsize ? gs1 : gs1-1; if(ts0[typeind]>mp->maxs0) mp->maxs0=ts0[typeind]; if(ts1[typeind]>mp->maxs1) mp->maxs1=ts1[typeind]; for(chi=0;chi1 && lasts0!=meshsize) { typeind=numtypes++; ts0[typeind] = lasts0; ts1[typeind] = meshsize; lastj = lasts1==meshsize ? gs1 : gs1-1; if(ts0[typeind]>mp->maxs0) mp->maxs0=ts0[typeind]; if(ts1[typeind]>mp->maxs1) mp->maxs1=ts1[typeind]; for(chi=0;chi1 && lasts1!=meshsize) { typeind=numtypes++; ts0[typeind] = meshsize; ts1[typeind] = lasts1; lasti = lasts0==meshsize ? gs0 : gs0-1; if(ts0[typeind]>mp->maxs0) mp->maxs0=ts0[typeind]; if(ts1[typeind]>mp->maxs1) mp->maxs1=ts1[typeind]; for(chi=0;chinmeshi-totalmeshcount==mp->nch) { typeind=numtypes++; ts0[typeind] = lasts0; ts1[typeind] = lasts1; if(ts0[typeind]>mp->maxs0) mp->maxs0=ts0[typeind]; if(ts1[typeind]>mp->maxs1) mp->maxs1=ts1[typeind]; for(chi=0;chinmeshi) error(EXIT_FAILURE, 0, "a bug! Please contact us at %s so we can fix " "it. The basic information for some meshes has not been found " "(in fillmeshinfo of mesh.c)", PACKAGE_BUGREPORT); } /* In the explanation below, all the parameters named are from the `struct gal_mesh_params` of `mesh.h`. An image contians `s0*s1` pixels in s0 rows and s1 columns. A mesh is a box of pixels within the image. A channel is defined as large regions of the image that should contain the meshes discussed above. So each channel contains a certain number of meshs and each mesh contains a certain number of pixels. In general, for any channel size, there can be four types of meshes. See the explanations above fillmeshinfo() for a more detailed discussion. So when all the channels have the same size, in the whole image, there can only be four types of meshes. The idea behind this classification is that CCDs often have more than one reading channel and essentially all the properties, vary from channel to channel. Therefore it is very important to do convolution, thresholding, detection and finding the sky background and noise properties differently for each channel. Each mesh is treated independently in its thread, but when interpolation over the meshes is desired, only meshes in each channel should be interpolated over. */ void gal_mesh_make_mesh(struct gal_mesh_params *mp) { size_t meshsize=mp->meshsize, lasts0, lasts1; size_t i, chs0=mp->s0/mp->nch2, chs1=mp->s1/mp->nch1; /* Set the number of channels. */ mp->nch=mp->nch1*mp->nch2; /* Incase meshsize is larger than the channel sizes, make it equal to the smaller of the channel axis sizes. */ if(meshsize>chs0 || meshsize>chs1) mp->meshsize = meshsize = (chs0ts0[i]=mp->ts1[i]=0; /* Set the mesh grid height (gs0, number of rows) and width (gs1, number of columns) on each channel. Note that the channels are assumed to be identical in size, so these values are the same for all the channels. In case the remainder of the image side size and meshsize is larger than lastmeshfrac, add a new mesh. If it is smaller than that fraction, then the remainder should be merged with the last mesh in the row or column. */ if( (float)(chs0%meshsize) > mp->lastmeshfrac*(float)(meshsize) ) { mp->gs0 = chs0/meshsize + 1; lasts0 = chs0%meshsize; } else { mp->gs0 = chs0/meshsize; lasts0 = meshsize+chs0%meshsize; } if( (float)(chs1%meshsize) > mp->lastmeshfrac*(float)(meshsize) ) { mp->gs1 = chs1/meshsize + 1; lasts1 = chs1%meshsize; } else { mp->gs1 = chs1/meshsize; lasts1 = meshsize+chs1%meshsize; } mp->nmeshc=mp->gs0*mp->gs1; mp->nmeshi=mp->nmeshc*mp->nch; /* Allocate the arrays to keep all the mesh starting points and types. Irrespective of which channel they lie in. */ mp->cgarray1=mp->cgarray2=mp->fgarray1=mp->fgarray2=NULL; errno=0; mp->start=malloc(mp->nmeshi*sizeof *mp->start); if(mp->start==NULL) error(EXIT_FAILURE, errno, "mesh starting points"); errno=0; mp->types=malloc(mp->nmeshi*sizeof *mp->types); if(mp->types==NULL) error(EXIT_FAILURE, errno, "mesh types"); errno=0; mp->chindex=malloc(mp->nmeshi*sizeof *mp->chindex); if(mp->chindex==NULL) error(EXIT_FAILURE, errno, "mesh in channel index"); errno=0; mp->imgindex=malloc(mp->nmeshi*sizeof *mp->imgindex); if(mp->imgindex==NULL) error(EXIT_FAILURE, errno, "mesh in image index"); /* Distribute the meshes in all the threads. */ gal_threads_dist_in_threads(mp->nmeshi, mp->numthreads, &mp->indexs, &mp->thrdcols); /* Fill in the information for each mesh and each type. */ fillmeshinfo(mp, chs0, chs1, lasts0, lasts1); } void gal_mesh_free_mesh(struct gal_mesh_params *mp) { free(mp->start); free(mp->types); free(mp->indexs); free(mp->chindex); free(mp->cgarray1); free(mp->cgarray2); free(mp->fgarray1); free(mp->fgarray2); free(mp->imgindex); } /*********************************************************************/ /******************** Mesh operations ********************/ /*********************************************************************/ /* The purpose of this function is to prepare the (possibly) multi-threaded environemnt, spin-off each thread and wait for them to finish for any operation that is to be done on the mesh grid. The arguments are: 1. A pointer to the gal_mesh_params structure that keeps all the information. 2. A pointer to a function that returns and gets a `void *' as its only argument. This function will be directly given to pthread_create. Through this argument, you can choose the function to operate on the mesh grid. 3. The size of each element to copy the mesh grid into, this has to be type size of the same type that constitutes `img' in gal_mesh_params. If the value to this argument is non-zero, an array will be allocated that can contain all the pixels in all the meshs and can be used by threads to manipute the pixels (for example sort them) in each mesh. 4. If the value of this argument is 1, then a second garray will be allocated in case your operation needs it. 5. Wether the allocated garrays should be initialized or not. */ void gal_mesh_operate_on_mesh(struct gal_mesh_params *mp, void *(*meshfunc)(void *), size_t oneforallsize, int makegarray2, int initialize) { int err; size_t i, nb; float *f, *fp; pthread_t t; /* We don't use the thread id, so all are saved here. */ pthread_attr_t attr; struct gal_mesh_thread_params *mtp; size_t numthreads=mp->numthreads; /* Allocate the arrays to keep the thread and parameters for each thread. */ errno=0; mtp=malloc(numthreads*sizeof *mtp); if(mtp==NULL) error(EXIT_FAILURE, errno, "%zu bytes in fillmesh (mesh.c) for mtp", numthreads*sizeof *mtp); /* Set the number of garrays to operate on: */ mp->ngarrays = makegarray2 ? 2 : 1; /* If cgarrays have not been allocated before, allocate them. */ if(mp->cgarray1==NULL) { errno=0; mp->cgarray1=malloc(mp->nmeshi*sizeof *mp->cgarray1); if(mp->cgarray1==NULL) error(EXIT_FAILURE, errno, "mp->cgarray1"); } if(mp->ngarrays==2 && mp->cgarray2==NULL) { errno=0; mp->cgarray2=malloc(mp->nmeshi*sizeof *mp->cgarray2); if(mp->cgarray2==NULL) error(EXIT_FAILURE, errno, "mp->cgarray2"); } /* Initialize the cgarrays to NaN:*/ if(initialize) { fp=(f=mp->cgarray1)+mp->nmeshi; do *f++=NAN; while(fngarrays==2) { fp=(f=mp->cgarray2)+mp->nmeshi; do *f++=NAN; while(fgarray1=mp->cgarray1; mp->garray2=mp->cgarray2; } /* `oneforall' is an array with the sides equal to the maximum side of the meshes in the image. The purpose is to enable manipulating the mesh pixels (for example sorting them and so on.). One such array is allocated for each thread in this one full allocation. Each thread can then use its own portion of this array through the following declaration: float *oneforall=&mp->oneforall[mtp->id*mp->maxs0*mp->maxs1]; In gal_mesh_params, `oneforall' is defined as a `void *', so the caller function, can cast it to any type it wants. The size of each type is given to `fillmesh' through the `oneforallsize' argument. */ if(oneforallsize) { errno=0; mp->oneforall=malloc(numthreads*mp->maxs0*mp->maxs1*oneforallsize); if(mp->oneforall==NULL) error(EXIT_FAILURE, errno, "unable to allocate %zu bytes for" "mtp->oneforall in fillmesh of mesh.c", numthreads*mp->maxs0*mp->maxs1*oneforallsize); } /* Spin off the threads: */ if(numthreads==1) { mtp[0].id=0; mtp[0].mp=mp; (*meshfunc)(&mtp[0]); } else { /* Initialize the attributes. Note that this running thread (that spinns off the nt threads) is also a thread, so the number the barrier should be one more than the number of threads spinned off. */ if(mp->nmeshinmeshi+1; else nb=numthreads+1; gal_threads_attr_barrier_init(&attr, &mp->b, nb); /* Spin off the threads: */ for(i=0;iindexs[i*mp->thrdcols]!=GAL_THREADS_NON_THRD_INDEX) { mtp[i].id=i; mtp[i].mp=mp; err=pthread_create(&t, &attr, meshfunc, &mtp[i]); if(err) error(EXIT_FAILURE, 0, "can't create thread %zu", i); } /* Wait for all threads to finish and free the spaces. */ pthread_barrier_wait(&mp->b); pthread_attr_destroy(&attr); pthread_barrier_destroy(&mp->b); } free(mtp); if(oneforallsize) free(mp->oneforall); } /*********************************************************************/ /******************** Interpolate ********************/ /*********************************************************************/ static void preparemeshinterparrays(struct gal_mesh_params *mp) { size_t bs0=mp->gs0, bs1=mp->gs1; size_t numthreads=mp->numthreads; /* If full-interpolation is to be done (ignoring channels) we will need two arrays to temporarily keep the actual positions of the meshs. Note that by default, the meshs in each channels are placed contiguously. In these arrays, the meshs are placed as they would in the image (channels are ignored).*/ if(mp->fullinterpolation) { /* In case the previous operation was on cgarrays, then you have to fill in fgarray. */ if(mp->garray1==mp->cgarray1) gal_mesh_full_garray(mp, 0); bs0=mp->nch2*mp->gs0; bs1=mp->nch1*mp->gs1; mp->garray1=mp->fgarray1; if(mp->ngarrays==2) mp->garray2=mp->fgarray2; } else { mp->garray1=mp->cgarray1; if(mp->ngarrays==2) mp->garray2=mp->cgarray2; } /* Allocate the output arrays to keep the final values. Note that we cannot just do the interpolaton on the same input grid, because the newly filled interpolated pixels will affect the later ones. In the end, these copies are going to replace the garrays. */ errno=0; mp->outgarray1=malloc(mp->nmeshi*sizeof *mp->outgarray1); if(mp->outgarray1==NULL) error(EXIT_FAILURE, errno, "%zu bytes for outgarray1 (mesh.c)", mp->nmeshi*sizeof *mp->outgarray1); if(mp->ngarrays==2) { errno=0; mp->outgarray2=malloc(mp->nmeshi*sizeof *mp->outgarray2); if(mp->outgarray2==NULL) error(EXIT_FAILURE, errno, "%zu bytes for outgarray2 (mesh.c)", mp->nmeshi*sizeof *mp->outgarray2); } /* Allocate the array for the values of the nearest pixels. For each pixel in each thread, the nearest pixels will be put here and sorted to find the median value. If garray2 is not NULL, then it should be interpolated. Note that both arrays have blank pixels on the same places.*/ errno=0; mp->nearest1=malloc(numthreads*mp->numnearest*sizeof *mp->nearest1); if(mp->nearest1==NULL) error(EXIT_FAILURE, errno, "%zu bytes for the array to keep the " "nearest1 values for interpolation (mesh.c)", numthreads*mp->numnearest*sizeof *mp->nearest1); if(mp->ngarrays==2) { errno=0; mp->nearest2=malloc(numthreads*mp->numnearest*sizeof *mp->nearest2); if(mp->nearest2==NULL) error(EXIT_FAILURE, errno, "%zu bytes for the array to keep the " "nearest2 values for interpolation (mesh.c)", numthreads*mp->numnearest*sizeof *mp->nearest2); } /* Allocate space for the byte array keeping a record of which pixels were used to search. Note that each thread needs one byt array. */ errno=0; mp->byt=malloc(numthreads*bs0*bs1*sizeof *mp->byt); if(mp->byt==NULL) error(EXIT_FAILURE, errno, "%zu bytes for mp->byt array in " "mesh.c", numthreads*bs0*bs1*sizeof *mp->byt); } /* Ideally, this should be a radial distance using the square root of the differences. But here we are not dealing with subpixel distances, so manhattan distance is fine. It also avoids the square root function which is much slower. */ static float manhattandistance(long ind, long xc, long yc, long s1) { return labs(ind%s1 - xc) + labs(ind/s1 - yc); } /* Some of the variables have different names than the gal_mesh_params structure because they are to be fed into the GAL_NEIGHBORS_FILL_4_ALLIMG macro. */ static void * meshinterponthread(void *inparams) { struct gal_mesh_thread_params *mtp=(struct gal_mesh_thread_params *)inparams; struct gal_mesh_params *mp=mtp->mp; /* Basic variables used in other definitions: */ size_t numnearest=mp->numnearest; size_t is0=mp->fullinterpolation ? mp->gs0*mp->nch2 : mp->gs0; size_t is1=mp->fullinterpolation ? mp->gs1*mp->nch1 : mp->gs1; /* Variables for this function: */ struct gal_linkedlist_tosll *lQ, *sQ; int ngarrays=mp->ngarrays; size_t xc, yc, *n, *nf, currentnum, thisind; unsigned char *byt=&mp->byt[mtp->id*is0*is1]; float *nearest1=&mp->nearest1[mtp->id*numnearest]; size_t i, *indexs=&mp->indexs[mtp->id*mp->thrdcols]; float mdist, *garray1=mp->garray1, *garray2=mp->garray2; size_t fmeshid, position, *ind=&position, numngb, ngb[4]; float *outgarray1=mp->outgarray1, *outgarray2=mp->outgarray2; float *nearest2 = ngarrays==2 ? &mp->nearest2[mtp->id*numnearest] : NULL; /* Go over all the meshes for this thread. */ for(i=0;indexs[i]!=GAL_THREADS_NON_THRD_INDEX;++i) { /* Get the index of this NaN mesh: */ thisind=indexs[i]; /* If this mesh is not blank and the user has only asked to interpolate blank pixels, then set the final values and go onto the next mesh. */ if(mp->interponlyblank && !isnan(garray1[thisind])) { outgarray1[thisind]=garray1[thisind]; if(ngarrays==2) outgarray2[thisind]=garray2[thisind]; continue; } /* Reset the byt array: */ memset(byt, 0, is0*is1); /* `fmeshid' (first-mesh-id) keeps the index of the first mesh in this channel. We are going to consider each channel as a sparate image for the neighbor finding job. This is why the pixels in each channel were designed to be contiguous. When we want to look at the value on each mesh, we simply sum its channel index with fmeshid. From this point on, *ind corresponds to the index of the mesh in the channel. We will also only be concerened with the portion of `mp->byt' array that is within this channel. So the `byt' pointer is set to point to the first mesh index in this channel. */ lQ=sQ=NULL; fmeshid = ( mp->fullinterpolation ? 0 : (thisind/mp->nmeshc) * mp->nmeshc); /* Initialize the necessary parameters. */ *ind=thisind-fmeshid; xc=*ind%is1; yc=*ind/is1; byt[*ind]=1; currentnum=0; gal_linkedlist_add_to_tosll_end( &lQ, &sQ, *ind, 0 ); /* Start finding the nearest filled pixels. */ while(sQ) { /* Pop out a pixel index (p) from the queue: */ gal_linkedlist_pop_from_tosll_start(&lQ, &sQ, ind, &mdist); /* If it isn't a NaN, then put it in the `nearest1' and `nearest2' arrays. */ if(!isnan(garray1[*ind+fmeshid])) { nearest1[currentnum]=garray1[*ind+fmeshid]; if(ngarrays==2) nearest2[currentnum]=garray2[*ind+fmeshid]; if(++currentnum>=numnearest) break; } /* Check the four neighbors and if they have not already been checked, put them into the queue. */ GAL_NEIGHBORS_FILL_4_ALLIMG; nf=(n=ngb)+numngb; do if(byt[*n]==0) { byt[*n]=1; gal_linkedlist_add_to_tosll_end(&lQ, &sQ, *n, manhattandistance(*n, xc, yc, is1)); } while(++n=numnearest' check above. */ if(sQ==NULL) error(EXIT_FAILURE, 0, "%s: only %zu mesh(s) are filled for " "interpolation in channel %zu. Either set less " "restrictive requirements to get more interpolation " "points or decrease the number of nearest points to " "use for interpolation. Problem encountered on thread " "%zu, for pixel %zu. When running on multiple threads, " "This message might be repeated for different threads", mp->errstart, currentnum, thisind/mp->nmeshc, mtp->id, thisind); } gal_linkedlist_tosll_free(lQ); /* Rest of the queue not needed. */ /* Find the median of the nearest neighbors and put it in: */ qsort(nearest1, numnearest, sizeof *nearest1, gal_qsort_float_increasing); outgarray1[thisind] = ( numnearest%2 ? nearest1[numnearest/2] : /* Odd. */ (nearest1[numnearest/2] /* Even. */ +nearest1[numnearest/2-1])/2 ); if(ngarrays==2) { qsort(nearest2, numnearest, sizeof *nearest2, gal_qsort_float_increasing); outgarray2[thisind] = ( numnearest%2 ? nearest2[numnearest/2] : /* Odd. */ (nearest2[numnearest/2] /* Even. */ +nearest2[numnearest/2-1])/2 ); } } /* If there is more than one thread, wait until the others finish. */ if(mp->numthreads>1) pthread_barrier_wait(&mp->b); return NULL; } void gal_mesh_interpolate(struct gal_mesh_params *mp, char *errstart) { int err; pthread_t t; /* We don't use the thread id, so all are saved here. */ size_t i, nb; pthread_attr_t attr; struct gal_mesh_thread_params *mtp; size_t numthreads=mp->numthreads; /* Prepare all the gal_mesh_params arrays: */ mp->errstart=errstart; preparemeshinterparrays(mp); /* Allocate the arrays to keep the thread and parameters for each thread. */ errno=0; mtp=malloc(numthreads*sizeof *mtp); if(mtp==NULL) error(EXIT_FAILURE, errno, "%zu bytes in fillmesh (mesh.c) for mtp", numthreads*sizeof *mtp); /* Spin off the threads: */ if(numthreads==1) { mtp[0].id=0; mtp[0].mp=mp; meshinterponthread(&mtp[0]); } else { /* Initialize the attributes. Note that this running thread (that spinns off the nt threads) is also a thread, so the number the barrier should be one more than the number of threads spinned off. */ if(mp->nmeshinmeshi+1; else nb=numthreads+1; gal_threads_attr_barrier_init(&attr, &mp->b, nb); /* Spin off the threads: */ for(i=0;iindexs[i*mp->thrdcols]!=GAL_THREADS_NON_THRD_INDEX) { mtp[i].id=i; mtp[i].mp=mp; err=pthread_create(&t, &attr, meshinterponthread, &mtp[i]); if(err) error(EXIT_FAILURE, 0, "can't create thread %zu", i); } /* Wait for all threads to finish and free the spaces. */ pthread_barrier_wait(&mp->b); pthread_attr_destroy(&attr); pthread_barrier_destroy(&mp->b); } /* Replace garray1 and garray2 with outgarray1 and outgarray2 */ if(mp->fullinterpolation) { free(mp->fgarray1); mp->garray1=mp->fgarray1=mp->outgarray1; } else { free(mp->cgarray1); mp->garray1=mp->cgarray1=mp->outgarray1; } if(mp->ngarrays==2) { if(mp->fullinterpolation) { free(mp->fgarray2); mp->garray2=mp->fgarray2=mp->outgarray2; } else { free(mp->cgarray2); mp->garray2=mp->cgarray2=mp->outgarray2; } } mp->outgarray1=mp->outgarray2=NULL; /* For a check system("rm test.fits"); gal_fits_array_to_file("test.fits", "garray1", FLOAT_IMG, mp->garray1, mp->nch2*mp->gs0, mp->nch1*mp->gs1, 1, NULL, NULL, "mesh"); gal_fits_array_to_file("test.fits", "garray2", FLOAT_IMG, mp->garray2, mp->nch2*mp->gs0, mp->nch1*mp->gs1, 1, NULL, NULL, "mesh"); */ /* Clean up. */ free(mtp); free(mp->byt); free(mp->nearest1); if(mp->ngarrays==2) free(mp->nearest2); } /*********************************************************************/ /******************** Smooth ********************/ /*********************************************************************/ void gal_mesh_smooth(struct gal_mesh_params *mp) { float *charray; float *f, *o, *fp, *tmp, *kernel, *sgarray1, *sgarray2; size_t numthreads=mp->numthreads, gs0=mp->gs0, gs1=mp->gs1; size_t chid, nmeshc=mp->nmeshc, smoothwidth=mp->smoothwidth; /* Make the smoothing kernel and set all its elements to 1. */ errno=0; kernel=malloc(smoothwidth*smoothwidth*sizeof *kernel); if(kernel==NULL) error(EXIT_FAILURE, errno, "%zu bytes for kernel in mesh.c", mp->smoothwidth*sizeof *kernel); fp=(f=kernel)+smoothwidth*smoothwidth; do *f++=1; while(ffullsmooth) { /* In case the previous operation was on the cgarrays. garray2 should not be checked. garray1 and garray2 are always in sync during one operation. However, if a previous operation had set garray2 and this operation only uses garray1, then things are going to go wrong. So Based on the principle that garray1 and garray2 are always going to be in sync with each other, we don't the mp->garray2==mp->cgarray2 check should not be done. */ if(mp->garray1==mp->cgarray1) gal_mesh_full_garray(mp, 0); /* Do the spatial convolution */ gal_spatialconvolve_convolve(mp->fgarray1, gs0*mp->nch2, gs1*mp->nch1, kernel, smoothwidth, smoothwidth, numthreads, 1, &sgarray1); free(mp->fgarray1); mp->garray1=mp->fgarray1=sgarray1; if(mp->ngarrays==2) { gal_spatialconvolve_convolve(mp->fgarray2, gs0*mp->nch2, gs1*mp->nch1, kernel, smoothwidth, smoothwidth, mp->numthreads, 1, &sgarray2); free(mp->fgarray2); mp->garray2=mp->fgarray2=sgarray2; } } else for(chid=0;chidnch;++chid) /* Note that in this mode, we do not */ { /* Allocate anything :-). */ /* If the last operation was done on the full image, then mp->garray1==mp->fgarray1. Therefore, the mesh boxes in each channel will not be congituous. So we have to update cgarray and set mp->garray1=mp->cgarray1. */ if(mp->garray1==mp->fgarray1) gal_mesh_full_garray(mp, 1); mp->garray1=mp->cgarray1; mp->garray2=mp->cgarray2; charray=&mp->cgarray1[chid*nmeshc]; gal_spatialconvolve_convolve(charray, gs0, gs1, kernel, smoothwidth, smoothwidth, numthreads, 1, &tmp); o=tmp; fp=(f=charray)+gs0*gs1; do *f=*o++; while(++fngarrays==2) { charray=&mp->cgarray2[chid*nmeshc]; gal_spatialconvolve_convolve(charray, gs0, gs1, kernel, smoothwidth, smoothwidth, numthreads, 1, &tmp); o=tmp; fp=(f=charray)+gs0*gs1; do *f=*o++; while(++fmp; const size_t ks0=mp->ks0, ks1=mp->ks1, is1=mp->s1; double sum, ksum; const size_t *types=mp->types; size_t chid, *chbrd=mtp->chbrd, ystart; const size_t *ts0=mp->ts0, *ts1=mp->ts1; size_t i, meshid, ind, *start=mp->start; size_t x, y, fx, fy, a, b, k0h=ks0/2, k1h=ks1/2; size_t xmin, xmax, ymin, ymax, nmeshc=mp->nmeshc; size_t *indexs=&mp->indexs[mtp->id*mp->thrdcols]; float *img=mp->img, *conv=mtp->conv, *kernel=mp->kernel; /* For each mesh in this thread, convolve the mesh */ for(i=0; (meshid=indexs[i])!=GAL_THREADS_NON_THRD_INDEX; ++i) { /* Get the channel ID and the relevant information for this mesh. */ chid=meshid/nmeshc; xmin=chbrd[chid*4]+k0h; /* Within these four points, the */ xmax=chbrd[chid*4+2]-k0h; /* convolution does not have to worry */ ymin=chbrd[chid*4+1]+k1h; /* about the edges. */ ymax=chbrd[chid*4+3]-k1h; /* Get the starting and ending positions of this mesh. NOTE: ystart is needed because for every `x', the value of y needs to change. */ fx = ( x = start[meshid]/is1 ) + ts0[types[meshid]]; fy = ( ystart = start[meshid]%is1 ) + ts1[types[meshid]]; /* If the mesh is on the edge of the channel it should be treated differently compared to when it is not. */ if( x>=xmin && ystart>=ymin && fx=xmin && y>=ymin && fx=xmin && x+a=ymin && y+bnumthreads>1) pthread_barrier_wait(&mp->b); return NULL; } void gal_mesh_spatial_convolve_on_mesh(struct gal_mesh_params *mp, float **conv) { int err; pthread_t t; /* We don't use the thread id, so all are saved here. */ pthread_attr_t attr; size_t i, nb, *chbrd; struct gal_mesh_thread_params *mtp; size_t numthreads=mp->numthreads; /* Allocate the arrays to keep the thread and parameters for each thread. */ errno=0; mtp=malloc(numthreads*sizeof *mtp); if(mtp==NULL) error(EXIT_FAILURE, errno, "%zu bytes in fillmesh (mesh.c) for mtp", numthreads*sizeof *mtp); /* Allocate space for the convolved array. */ errno=0; *conv=malloc(mp->s0*mp->s1* sizeof **conv); if(*conv==NULL) error(EXIT_FAILURE, errno, "%zu bytes for convolution on mesh output", mp->s0*mp->s1* sizeof **conv); /* Channel borders so we can see if a mesh is inside or outside a channel. chbrd contians for number for each channel: in order they are: 1. The channel's first pixel's first C axis value. 2. The channel's first pixel's second C axis value. 3. The channel's last pixel's first C axis value. 4. The channel's last pixel's second C axis value. */ errno=0; chbrd=malloc(mp->nch*4*sizeof *chbrd); if(chbrd==NULL) error(EXIT_FAILURE, errno, "%zu bytes for chbrd in " "gal_mesh_spatial_convolve_on_mesh", mp->nch*4*sizeof *chbrd); for(i=0;inch;++i) { if(mp->fullconvolution) { chbrd[i*4+2]=mp->s0; chbrd[i*4+3]=mp->s1; chbrd[i*4]=chbrd[i*4+1]=0; } else { chbrd[i*4+0]=mp->start[i*mp->nmeshc]/mp->s1; chbrd[i*4+1]=mp->start[i*mp->nmeshc]%mp->s1; chbrd[i*4+2]=chbrd[i*4+0]+mp->s0/mp->nch2; chbrd[i*4+3]=chbrd[i*4+1]+mp->s1/mp->nch1; } } /* Spin off the threads: */ if(numthreads==1) { mtp[0].id=0; mtp[0].mp=mp; mtp[0].conv=*conv; mtp[0].chbrd=chbrd; meshspatialconvonthreads(&mtp[0]); } else { /* Initialize the attributes. Note that this running thread (that spinns off the nt threads) is also a thread, so the number the barrier should be one more than the number of threads spinned off. */ if(mp->nmeshinmeshi+1; else nb=numthreads+1; gal_threads_attr_barrier_init(&attr, &mp->b, nb); /* Spin off the threads: */ for(i=0;iindexs[i*mp->thrdcols]!=GAL_THREADS_NON_THRD_INDEX) { mtp[i].id=i; mtp[i].mp=mp; mtp[i].conv=*conv; mtp[i].chbrd=chbrd; err=pthread_create(&t, &attr, meshspatialconvonthreads, &mtp[i]); if(err) error(EXIT_FAILURE, 0, "can't create thread %zu", i); } /* Wait for all threads to finish and free the spaces. */ pthread_barrier_wait(&mp->b); pthread_attr_destroy(&attr); pthread_barrier_destroy(&mp->b); } free(mtp); free(chbrd); } /* The indexs array for correcting the convolution on inner channel edges has been allocated. Note that gal_threads_dist_in_threads will distribute indexs from zero to numpix-1. After it, we should fill in all the channels. The method of filling in the indexs array with the proper indexs to re-convolve is very similar to the method explained below in gal_mesh_change_to_full_convolution, where it is explained how to count the number of pixels that should be re-convolved. */ static void corrconvindexs(struct gal_mesh_params *mp, size_t **indexs, size_t *numpix, size_t *thrdcols) { size_t i, j, a, b; size_t numthreads=mp->numthreads; size_t alow, ahigh, blow, bhigh, *ind; size_t npch0=mp->s0/mp->nch2, npch1=mp->s1/mp->nch1; size_t nch1=mp->nch1, nch2=mp->nch2, ks0=mp->ks0, ks1=mp->ks1; size_t s0=mp->s0, s1=mp->s1, hk0=mp->ks0/2+1, hk1=mp->ks1/2+1; /* Find the number of pixels that must be convolved. Note that when we don't care about the edges, on each dimension, we have one less border than the number of channels in that dimention. On each channel's border, we want to re-convolve the ks0/2+1 pixels before the channel edge along the first dimension. So in total, for each channel edge, we want ks0+1 pixels on its two sides. Don't forget that the kernel sides are odd. So on the first dimension, we have (ks0+1)*(nch2-1) pixels that should be re-convolved. Multiplying it by s1, we get the total number of pixels in 2D around the first axis internal edges. Along the second dimension, we have (ks1+1)*(nch1-1) pixels. But this time we can't just multiply by s0 to get the total number of 2D pixels. Because of the overlap. So we only have to multily by the number of rows that were not accounted in the first run, which is s0-(ks0+1)*(nch2-1). */ *numpix = ( (ks0+1)*(nch2-1)*s1 + (ks1+1)*(nch1-1)*(s0-(ks0+1)*(nch2-1)) ); /* Distribute the indexs of the desired pixels into the indexs array. */ gal_threads_dist_in_threads(*numpix, numthreads, indexs, thrdcols); ind=*indexs; for(i=1;is0 ? s0 : i*npch0+hk0; /* For a check printf("1: alow: %-4zu ahigh: %-4zu.\t(0 -- %zu)\n", alow, ahigh, s1); */ for(a=alow; as1 ? s1 : j*npch1+hk1; for(b=blow; bs0 ? s0 : i*npch0+hk0; } /* All the areas under were checked, now we have to add the area ontop of the highest middle channel edge. Note that when there is no channel along the first C axis (nch2==1), then it will immediately come here and scan all the rows between the blow and bhigh columns. */ ahigh=s0; /* For a check: printf("3: alow: %-4zu ahigh: %-4zu. b: %-10zu (%zu -- %zu)\n", alow, ahigh, b, blow, bhigh); */ for(a=alow;anch==1 || mp->fullconvolution) return; mp->fullconvolution=1; /* Array keeping thread parameters for each thread.*/ errno=0; scp=malloc(mp->numthreads*sizeof *scp); if(scp==NULL) error(EXIT_FAILURE, errno, "%zu bytes for scp in gal_mesh_change_to_full_convolution " "(mesh.c)", mp->numthreads*sizeof *scp); /* Put the indexs of the pixels to re-convolve here. */ corrconvindexs(mp, &indexs, &numpix, &thrdcols); /* Start the convolution on the desired pixels. */ if(mp->numthreads==1) { gal_spatialconvolve_pparams(mp->img, mp->s0, mp->s1, mp->kernel, mp->ks0, mp->ks1, mp->numthreads, 1, conv, indexs, &scp[0]); gal_spatialconvolve_thread(&scp[0]); } else { /* Initialize the attributes. Note that this running thread (that spinns off the nt threads) is also a thread, so the number the barrier should be one more than the number of threads spinned off. */ if(numpixnumthreads) nb=numpix+1; else nb=mp->numthreads+1; gal_threads_attr_barrier_init(&attr, &b, nb); /* Spin off the threads: */ for(i=0;inumthreads;++i) if(indexs[i*thrdcols]!=GAL_THREADS_NON_THRD_INDEX) { scp[i].b=&b; gal_spatialconvolve_pparams(mp->img, mp->s0, mp->s1, mp->kernel, mp->ks0, mp->ks1, mp->numthreads, 1, conv, &indexs[i*thrdcols], &scp[i]); err=pthread_create(&t, &attr, gal_spatialconvolve_thread, &scp[i]); if(err) error(EXIT_FAILURE, 0, "can't create thread %zu", i); } /* Wait for all threads to finish and free the spaces. */ pthread_barrier_wait(&b); pthread_attr_destroy(&attr); pthread_barrier_destroy(&b); } free(scp); free(indexs); } gnuastro-0.2.33-8a3b/lib/linkedlist.c0000644000175000017500000003523013001632540014166 00000000000000/********************************************************************* Functions for linked lists. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include /**************************************************************** ***************** Float ******************** ****************************************************************/ void gal_linkedlist_print_fll_array(struct gal_linkedlist_fll **afll, size_t num) { size_t i; struct gal_linkedlist_fll *tmp; for(i=0;inext) printf("%f, ", tmp->v); printf("\n"); } } void gal_linkedlist_add_to_fll(struct gal_linkedlist_fll **list, float value) { struct gal_linkedlist_fll *newnode; errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "linkedlist: New element in " "gal_linkedlist_fll"); newnode->v=value; newnode->next=*list; *list=newnode; } void gal_linkedlist_pop_from_fll(struct gal_linkedlist_fll **list, float *value) { struct gal_linkedlist_fll *tmp; tmp=*list; *value=tmp->v; *list=tmp->next; free(tmp); } size_t gal_linkedlist_num_in_fll(struct gal_linkedlist_fll *list) { size_t num=0; struct gal_linkedlist_fll *tmp; for(tmp=list;tmp!=NULL;tmp=tmp->next) ++num; return num; } void gal_linkedlist_fll_to_array(struct gal_linkedlist_fll *list, float **f, size_t *num) { float *tf; size_t i=0; struct gal_linkedlist_fll *tmp; /* Find the number of elements: */ if(*num==0) *num=gal_linkedlist_num_in_fll(list); /* Allocate the space: */ errno=0; *f=malloc(*num*sizeof(float)); if(*f==NULL) error(EXIT_FAILURE, errno, "linkedlist: array of gal_linkedlist_fll " "with %zu elements", *num); tf=*f; /* Fill in the array: */ for(tmp=list;tmp!=NULL;tmp=tmp->next) tf[i++]=tmp->v; } void gal_linkedlist_free_fll(struct gal_linkedlist_fll *list) { struct gal_linkedlist_fll *tmp, *ttmp; tmp=list; while(tmp!=NULL) { ttmp=tmp->next; free(tmp); tmp=ttmp; } } void gal_linkedlist_free_fll_array(struct gal_linkedlist_fll **afll, size_t num) { size_t i; for(i=0;ia=a; newnode->b=b; newnode->next=*list; *list=newnode; } void gal_linkedlist_pop_from_tdll(struct gal_linkedlist_tdll **list, double *a, double *b) { struct gal_linkedlist_tdll *tmp=*list; *a=tmp->a; *b=tmp->b; *list=tmp->next; free(tmp); } size_t gal_linkedlist_num_int_dll(struct gal_linkedlist_tdll *list) { size_t num=0; struct gal_linkedlist_tdll *tmp; for(tmp=list;tmp!=NULL;tmp=tmp->next) ++num; return num; } void gal_linkedlist_tdll_to_array_inv(struct gal_linkedlist_tdll *list, double **d, size_t *num) { size_t i; double *td; struct gal_linkedlist_tdll *tmp; /* Find the number of elements: */ if(*num==0) *num=gal_linkedlist_num_int_dll(list); /* Allocate the space (every element of the list has two elements.) */ errno=0; td=*d=malloc(2 * *num * sizeof(double)); if(*d==NULL) error(EXIT_FAILURE, errno, "linkedlist: array of gal_linkedlist_tdll " "with %zu elements", *num); /* Fill in the array in reverse order */ i = 2 * *num - 2; for(tmp=list;tmp!=NULL;tmp=tmp->next) { td[i]=tmp->a; td[i+1]=tmp->b; i-=2; } } void gal_linkedlist_free_tdll(struct gal_linkedlist_tdll *list) { struct gal_linkedlist_tdll *tmp, *ttmp; tmp=list; while(tmp!=NULL) { ttmp=tmp->next; free(tmp); tmp=ttmp; } } /**************************************************************** ***************** string ******************** ****************************************************************/ void gal_linkedlist_add_to_stll(struct gal_linkedlist_stll **list, char *value) { struct gal_linkedlist_stll *newnode; errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "linkedlist: New element in gal_linkedlist_stll"); newnode->v=value; newnode->next=*list; *list=newnode; } void gal_linkedlist_pop_from_stll(struct gal_linkedlist_stll **list, char **value) { struct gal_linkedlist_stll *tmp; tmp=*list; *value=tmp->v; *list=tmp->next; free(tmp); } void gal_linkedlist_reverse_stll(struct gal_linkedlist_stll **list) { char *thisstring; struct gal_linkedlist_stll *correctorder=NULL; while(*list!=NULL) { gal_linkedlist_pop_from_stll(list, &thisstring); gal_linkedlist_add_to_stll(&correctorder, thisstring); } *list=correctorder; } void gal_linkedlist_print_stll(struct gal_linkedlist_stll *list) { struct gal_linkedlist_stll *tmp; for(tmp=list; tmp!=NULL; tmp=tmp->next) printf("%s\n", tmp->v); } size_t gal_linkedlist_num_in_stll(struct gal_linkedlist_stll *list) { size_t num=0; struct gal_linkedlist_stll *tmp; for(tmp=list;tmp!=NULL;tmp=tmp->next) ++num; return num; } /**************************************************************** ***************** size_t ******************** ****************************************************************/ void gal_linkedlist_add_to_sll(struct gal_linkedlist_sll **list, size_t value) { struct gal_linkedlist_sll *newnode; errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "linkedlist: New element in gal_linkedlist_sll"); newnode->v=value; newnode->next=*list; *list=newnode; } void gal_linkedlist_pop_from_sll(struct gal_linkedlist_sll **list, size_t *value) { struct gal_linkedlist_sll *tmp; tmp=*list; *value=tmp->v; *list=tmp->next; free(tmp); } size_t gal_linkedlist_num_in_sll(struct gal_linkedlist_sll *list) { size_t num=0; struct gal_linkedlist_sll *tmp; for(tmp=list;tmp!=NULL;tmp=tmp->next) ++num; return num; } void gal_linkedlist_sll_to_array(struct gal_linkedlist_sll *list, size_t **s, size_t *num, int inverse) { size_t i, *ts; struct gal_linkedlist_sll *tmp; *num=gal_linkedlist_num_in_sll(list); errno=0; *s=malloc(*num*sizeof(size_t)); if(*s==NULL) error(EXIT_FAILURE, errno, "linkedlist: array of gal_linkedlist_sll " "with %zu elements", *num); ts=*s; i = inverse ? *num-1: 0; if(inverse) for(tmp=list;tmp!=NULL;tmp=tmp->next) ts[i--]=tmp->v; else for(tmp=list;tmp!=NULL;tmp=tmp->next) ts[i++]=tmp->v; } void gal_linkedlist_print_sll(struct gal_linkedlist_sll *list) { struct gal_linkedlist_sll *tmp; printf("\n\n"); for(tmp=list;tmp!=NULL;tmp=tmp->next) printf("%zu, ", tmp->v); printf("\b\b.\n\n"); return; } void gal_linkedlist_free_sll(struct gal_linkedlist_sll *list) { struct gal_linkedlist_sll *tmp, *ttmp; tmp=list; while(tmp!=NULL) { ttmp=tmp->next; free(tmp); tmp=ttmp; } } /**************************************************************** ****************** Ordered SLL ******************** ***************** size_t ******************** ****************************************************************/ /* We want to put the nodes in order based on the 'tosort' value of each node. The top element should always have the smallest radius. */ void gal_linkedlist_add_to_osll(struct gal_linkedlist_osll **list, size_t value, float tosort) { struct gal_linkedlist_osll *newnode, *tmp=*list, *prev=NULL; errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "linkedlist: New element " "in gal_linkedlist_osll"); newnode->v=value; newnode->s=tosort; /* *list points to the smallest value in the queue!*/ while(tmp!=NULL) { if(tosorts) break; /* No need for else, it will only come here if the condition above is not satisfied. */ prev=tmp; tmp=tmp->next; } if(tmp==NULL) /* This is the largest value so far. */ { /* '*list' only changes if it is NULL. */ newnode->next=NULL; if(prev) prev->next=newnode; /* 'prev' is not NULL! */ else *list=newnode; /* Only for initial node. */ } else { if(prev) prev->next=newnode; else *list=newnode; /* 'tosort' is smaller than all. */ newnode->next=tmp; } } /* Note that the popped element is the smallest! */ void gal_linkedlist_pop_from_osll(struct gal_linkedlist_osll **list, size_t *value, float *sortvalue) { struct gal_linkedlist_osll *tmp; tmp=*list; *value=tmp->v; *sortvalue=tmp->s; *list=tmp->next; free(tmp); } /* Add the elements of an gal_linkedlist_osll to a gal_linkedlist_sll. */ void gal_linkedlist_osll_into_sll(struct gal_linkedlist_osll *in, struct gal_linkedlist_sll **out) { struct gal_linkedlist_osll *tmp; while(in!=NULL) { tmp=in->next; gal_linkedlist_add_to_sll(out, in->v); free(in); in=tmp; } } /**************************************************************** ****************** Two way, Ordered SLL ******************** ***************** size_t ******************** ****************************************************************/ /* The two way ordered SLL looks something like this: largest pointer | NULL <-- (v0,s0) <--> (v1,s1) <--> ... (vn,sn) --> NULL | smallest pointer Where s(n)>s(n+1) for all n. */ void gal_linkedlist_print_tosll(struct gal_linkedlist_tosll *largest, struct gal_linkedlist_tosll *smallest) { size_t counter=1; /* We are not counting array elements :-D ! */ while(largest!=NULL) { printf("\t%-5zu (%zu, %.4f) \n", counter++, largest->v, largest->s); largest=largest->next; printf("\t\t\t\t(%zu, %.4f)\n", smallest->v, smallest->s); smallest=smallest->prev; } printf("\n"); } /* Very similar to Ordered SLL, but now it is two way. */ void gal_linkedlist_add_to_tosll_end(struct gal_linkedlist_tosll **largest, struct gal_linkedlist_tosll **smallest, size_t value, float tosort) { struct gal_linkedlist_tosll *newnode, *tmp=*largest; errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "linkedlist: New element " "in gal_linkedlist_tosll"); newnode->v=value; newnode->s=tosort; newnode->prev=NULL; while(tmp!=NULL) { if(tosort >= tmp->s) break; /* No need for else, it will only come here if the condition above is not satisfied. */ newnode->prev=tmp; tmp=tmp->next; } if(tmp==NULL) /* This is the smallest value so far. */ { /* '*largest' only changes if it is NULL. */ newnode->next=NULL; *smallest=newnode; if(newnode->prev) /* 'prev' is not NULL! */ newnode->prev->next=newnode; else /* 'prev is NULL, Only first. */ *largest=newnode; } else { if(newnode->prev) { newnode->prev->next->prev=newnode; newnode->prev->next=newnode; } else { (*largest)->prev=newnode; *largest=newnode; /* 'tosort' is larger than all. */ } newnode->next=tmp; } } /* Note that start has to be initialized. */ void gal_linkedlist_pop_from_tosll_start(struct gal_linkedlist_tosll **largest, struct gal_linkedlist_tosll **smallest, size_t *value, float *tosort) { struct gal_linkedlist_tosll *tmp=*smallest; *value=tmp->v; *tosort=tmp->s; *smallest=tmp->prev; free(tmp); if(*smallest) (*smallest)->next=NULL; else *largest=NULL; /*printf("Popped v: %zu, s: %f\n", *value, *tosort);*/ } void gal_linkedlist_smallest_tosll(struct gal_linkedlist_tosll *largest, struct gal_linkedlist_tosll **smallest) { struct gal_linkedlist_tosll *tmp=largest; while(tmp!=NULL) { if(tmp->next==NULL) { *smallest=tmp; break; } tmp=tmp->next; } /* If *largest wasn't NULL initially, tmp should not be NULL because the loop terminated before it becomes null. But if it was initiall NULL, it will never enter the loop, and so smallest should also be NULL. */ if(tmp==NULL) *smallest=NULL; } void gal_linkedlist_tosll_into_sll(struct gal_linkedlist_tosll *in, struct gal_linkedlist_sll **out) { struct gal_linkedlist_tosll *tmp; while(in!=NULL) { tmp=in->next; gal_linkedlist_add_to_sll(out, in->v); free(in); in=tmp; } } void gal_linkedlist_tosll_free(struct gal_linkedlist_tosll *largest) { struct gal_linkedlist_tosll *tmp; while(largest!=NULL) { tmp=largest->next; free(largest); largest=tmp; } } gnuastro-0.2.33-8a3b/lib/git.c0000644000175000017500000000472113001632540012610 00000000000000/********************************************************************* Functions to deal with Git version controlled directories. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include /* Return the result of Git describe and */ char * gal_git_describe(void) { char *describe_return=NULL; /* Only actually work on Git if the library is present. */ #if GAL_GNUASTRO_HAVE_LIBGIT2 == 1 git_buf buf={0}; git_repository *repo; git_describe_result *describe_result; git_describe_format_options format_options; git_describe_options describe_options = GIT_DESCRIBE_OPTIONS_INIT; /* Initialize Git's global setup. */ git_libgit2_init(); /* Initialize the descriptions. */ git_describe_init_format_options(&format_options, GIT_DESCRIBE_FORMAT_OPTIONS_VERSION); /* Set some values manually: */ describe_options.show_commit_oid_as_fallback=1; format_options.dirty_suffix="-dirty"; /* Open the Git repository. */ if( !git_repository_open_ext(&repo, ".", 0, NULL) && !git_describe_workdir(&describe_result, repo, &describe_options) && !git_describe_format(&buf, describe_result, &format_options) ) { /* Allocate space for and copy the description. */ errno=0; describe_return=malloc(strlen(buf.ptr)+1); if(describe_return==NULL) error(EXIT_FAILURE, errno, "%zu bytes to copy Git's describe", strlen(buf.ptr)+1); strcpy(describe_return, buf.ptr); } /* Clean up. */ git_repository_free(repo); git_libgit2_shutdown(); #endif /* Return */ return describe_return; } gnuastro-0.2.33-8a3b/lib/fits.c0000644000175000017500000017541613002474472013015 00000000000000/********************************************************************* Functions to work with FITS image data. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include "checkset.h" #include "fixedstringmacros.h" /************************************************************* ************** Reporting errors: *************** *************************************************************/ void gal_fits_io_error(int status, char *message) { char defmessage[]="Error in CFITSIO, see above."; if(status) { fits_report_error(stderr, status); if(message) error(EXIT_FAILURE, 0, "%s", message); else error(EXIT_FAILURE, 0, "%s", defmessage); } } /************************************************************* ************** Acceptable FITS names *************** *************************************************************/ int gal_fits_name_is_fits(char *name) { size_t len; len=strlen(name); if ( ( len>=4 && strcmp(&name[len-4], "fits") == 0 ) || ( len>=7 && strcmp(&name[len-7], "fits.gz") == 0 ) || ( len>=6 && strcmp(&name[len-6], "fits.Z") == 0 ) || ( len>=3 && strcmp(&name[len-3], "imh") == 0 ) || ( len>=7 && strcmp(&name[len-7], "fits.fz") == 0 ) ) return 1; else return 0; } int gal_fits_suffix_is_fits(char *suffix) { if (strcmp(suffix, "fits") == 0 || strcmp(suffix, ".fits") == 0 || strcmp(suffix, "fits.gz") == 0 || strcmp(suffix, ".fits.gz") == 0 || strcmp(suffix, "fits.Z") == 0 || strcmp(suffix, ".fits.Z") == 0 || strcmp(suffix, "imh") == 0 || strcmp(suffix, ".imh") == 0 || strcmp(suffix, "fits.fz") == 0 || strcmp(suffix, ".fits.fz") == 0) return 1; else return 0; } /************************************************************* ************** BITPIX Dependancies *************** *************************************************************/ /* Set datatype (in CFITSIO) based on BITPIX. */ int gal_fits_bitpix_to_datatype(int bitpix) { switch(bitpix) { case BYTE_IMG: return TBYTE; case SHORT_IMG: return TSHORT; case LONG_IMG: return TLONG; case LONGLONG_IMG: return TLONGLONG; case FLOAT_IMG: return TFLOAT; case DOUBLE_IMG: return TDOUBLE; case SBYTE_IMG: return TSBYTE; case USHORT_IMG: return TUSHORT; case ULONG_IMG: return TULONG; default: error(EXIT_FAILURE, 0, "bitpix value of %d not recognized", bitpix); } return 0; } /* The values to the TFORM header keyword are single letter capital letters, but that is useless in identifying the data type of the column. So this function will do the conversion based on the CFITSIO manual.*/ int gal_fits_tform_to_datatype(char tform) { switch(tform) { case 'X': return TBIT; case 'B': return TBYTE; case 'L': return TLOGICAL; case 'A': return TSTRING; case 'I': return TSHORT; case 'J': return TLONG; case 'K': return TLONGLONG; case 'E': return TFLOAT; case 'D': return TDOUBLE; case 'C': return TCOMPLEX; case 'M': return TDBLCOMPLEX; case 'S': return TSBYTE; case 'V': return TUINT; case 'U': return TUSHORT; default: error(EXIT_FAILURE, 0, "'%c' is not a recognized CFITSIO value for " "the TFORMn header keyword(s).", tform); } error(EXIT_FAILURE, 0, "A bug! Please contact us so we can fix this. " "For some reason, control has reached to the end of the " "gal_fits_tform_to_datatype function in fits.c."); return -1; } void gal_fits_img_bitpix_size(fitsfile *fptr, int *bitpix, long *naxes) { int status=0, maxdim=10, naxis; if( fits_get_img_param(fptr, maxdim, bitpix, &naxis, naxes, &status) ) gal_fits_io_error(status, NULL); if(naxis!=2) error(EXIT_FAILURE, 0, "currently only a 2 dimensional image array " "is supported. Your array is %d dimension(s). %s", naxis, naxis ? "Please contact us to add this feature." : "This might " "Be due to the fact that the data in images with multiple " "extensions are sometimes put on the second extension. If this " "is the case, try changing the hdu (maybe to --hdu=1)"); } void * gal_fits_datatype_blank(int datatype) { /* Define the pointers, note that we are ordering them based on the CFITSIO manual to be more easily comparable. */ unsigned char *b; char *c; char **str; short *s; long *l; LONGLONG *L; float *f; double *d; gsl_complex_float *cx; gsl_complex *dcx; int *i; unsigned int *ui; unsigned short *us; unsigned long *ul; errno=0; switch(datatype) { case TBIT: error(EXIT_FAILURE, 0, "Currently Gnuastro doesn't support TBIT " "datatype, please get in touch with us to implement it."); case TBYTE: b=malloc(sizeof *b); if(b==NULL) error(EXIT_FAILURE, errno, "%zu bytes for blank TBYTE", sizeof *b); *b=GAL_FITS_BYTE_BLANK; return b; /* CFITSIO says "int for keywords, char for table columns". Here we are only assuming table columns. So in practice this also applies to TSBYTE.*/ case TLOGICAL: case TSBYTE: c=malloc(sizeof *c); if(c==NULL) error(EXIT_FAILURE, errno, "%zu bytes for blank TLOGICAL, or TSBYTE", sizeof *c); *c=GAL_FITS_LOGICAL_BLANK; return c; case TSTRING: str=malloc(sizeof *str); if(str==NULL) error(EXIT_FAILURE, errno, "%zu bytes for blank TSTRING", sizeof *s); *str=GAL_FITS_STRING_BLANK; return str; case TSHORT: s=malloc(sizeof *s); if(s==NULL) error(EXIT_FAILURE, errno, "%zu bytes for blank TSHORT", sizeof *s); *s=GAL_FITS_SHORT_BLANK; return s; case TLONG: l=malloc(sizeof *l); if(l==NULL) error(EXIT_FAILURE, errno, "%zu bytes for blank TLONG", sizeof *l); *l=GAL_FITS_LONG_BLANK; return l; case TLONGLONG: L=malloc(sizeof *L); if(L==NULL) error(EXIT_FAILURE, errno, "%zu bytes for blank TLONGLONG", sizeof *L); *L=GAL_FITS_LLONG_BLANK; return L; case TFLOAT: f=malloc(sizeof *f); if(f==NULL) error(EXIT_FAILURE, errno, "%zu bytes for blank TFLOAT", sizeof *f); *f=GAL_FITS_FLOAT_BLANK; return f; case TDOUBLE: d=malloc(sizeof *d); if(d==NULL) error(EXIT_FAILURE, errno, "%zu bytes for blank TDOUBLE", sizeof *d); *d=GAL_FITS_DOUBLE_BLANK; return d; case TCOMPLEX: cx=malloc(sizeof *cx); if(cx==NULL) error(EXIT_FAILURE, errno, "%zu bytes for blank TCOMPLEX", sizeof *cx); GSL_SET_COMPLEX(cx,GAL_FITS_FLOAT_BLANK,GAL_FITS_FLOAT_BLANK); return cx; case TDBLCOMPLEX: dcx=malloc(sizeof *dcx); if(dcx==NULL) error(EXIT_FAILURE, errno, "%zu bytes for blank TDBLCOMPLEX", sizeof *dcx); GSL_SET_COMPLEX(dcx,GAL_FITS_DOUBLE_BLANK,GAL_FITS_DOUBLE_BLANK); return dcx; case TINT: i=malloc(sizeof *i); if(i==NULL) error(EXIT_FAILURE, errno, "%zu bytes for blank TINT", sizeof *i); *i=GAL_FITS_INT_BLANK; return i; case TUINT: ui=malloc(sizeof *ui); if(ui==NULL) error(EXIT_FAILURE, errno, "%zu bytes for blank TUINT", sizeof *ui); *ui=GAL_FITS_UINT_BLANK; return ui; case TUSHORT: us=malloc(sizeof *us); if(us==NULL) error(EXIT_FAILURE, errno, "%zu bytes for blank TUSHORT", sizeof *us); *us=GAL_FITS_USHORT_BLANK; return us; case TULONG: ul=malloc(sizeof *ul); if(ul==NULL) error(EXIT_FAILURE, errno, "%zu bytes for blank TULONG", sizeof *ul); *ul=GAL_FITS_ULONG_BLANK; return ul; default: error(EXIT_FAILURE, 0, "datatype value of %d not recognized", datatype); } return NULL; } /* Allocate an array based on the value of datatype. Note that the argument `size' is the number of elements, necessary in the array, the number of bytes each element needs will be determined internaly by this function using the datatype argument, so you don't have to worry about it. */ void * gal_fits_datatype_alloc(size_t size, int datatype) { void *array; /* Allocate space for the array to keep the image. */ switch(datatype) { case TBIT: error(EXIT_FAILURE, 0, "Currently Gnuastro doesn't support TBIT " "datatype, please get in touch with us to implement it."); /* The parenthesis after sizeof is not a function, it is actually a type cast, so we have put a space between size of and the parenthesis to highlight this. In C, `sizeof' is an operator, not a function.*/ case TBYTE: size *= sizeof (unsigned char); break; case TLOGICAL: case TSBYTE: size *= sizeof (char); break; case TSTRING: size *= sizeof (char *); break; case TSHORT: size *= sizeof (short); break; case TLONG: size *= sizeof (long); break; case TLONGLONG: size *= sizeof (LONGLONG); break; case TFLOAT: if( sizeof (float) != 4 ) error(EXIT_FAILURE, 0, "`float` is not 32bits on this machine. The FITS standard " "Requires this size"); size *= sizeof (float); break; case TDOUBLE: if( sizeof (double) != 8 ) error(EXIT_FAILURE, 0, "`double` is not 64bits on this machine. The FITS standard " "requires this size"); size *= sizeof (double); break; case TCOMPLEX: if( sizeof (float) != 4 ) error(EXIT_FAILURE, 0, "`float` is not 32bits on this machine. The FITS standard " "Requires this size"); size *= sizeof (gsl_complex_float); break; case TDBLCOMPLEX: if( sizeof (double) != 8 ) error(EXIT_FAILURE, 0, "`double` is not 64bits on this machine. The FITS standard " "requires this size"); size *= sizeof (gsl_complex); break; case TINT: size *= sizeof (int); break; case TUINT: size *= sizeof (unsigned int); break; case TUSHORT: size *= sizeof (unsigned short); break; case TULONG: size *= sizeof (unsigned long); break; default: error(EXIT_FAILURE, 0, "datatype value of %d not recognized in " "gal_fits_datatype_alloc", datatype); } errno=0; array=malloc(size); if(array==NULL) error(EXIT_FAILURE, errno, "array of %zu bytes in gal_fits_datatype_alloc", size); return array; } size_t gal_fits_datatype_size(int datatype) { switch(datatype) { case TBIT: error(EXIT_FAILURE, 0, "Currently Gnuastro doesn't support TBIT " "datatype, please get in touch with us to implement it."); /* The parenthesis after sizeof is not a function, it is actually a type cast, so we have put a space between size of and the parenthesis to highlight this. In C, `sizeof' is an operator, not a function.*/ case TBYTE: return sizeof (unsigned char); case TLOGICAL: case TSBYTE: return sizeof (char); case TSTRING: return sizeof (char *); case TSHORT: return sizeof (short); case TLONG: return sizeof (long); case TLONGLONG: return sizeof (LONGLONG); case TFLOAT: if( sizeof (float) != 4 ) error(EXIT_FAILURE, 0, "`float` is not 32bits on this machine. The FITS standard " "Requires this size"); return sizeof (float); case TDOUBLE: if( sizeof (double) != 8 ) error(EXIT_FAILURE, 0, "`double` is not 64bits on this machine. The FITS standard " "requires this size"); return sizeof (double); case TCOMPLEX: if( sizeof (float) != 4 ) error(EXIT_FAILURE, 0, "`float` is not 32bits on this machine. The FITS standard " "Requires this size"); return sizeof (gsl_complex_float); case TDBLCOMPLEX: if( sizeof (double) != 8 ) error(EXIT_FAILURE, 0, "`double` is not 64bits on this machine. The FITS standard " "requires this size"); return sizeof (gsl_complex); case TINT: return sizeof (int); case TUINT: return sizeof (unsigned int); case TUSHORT: return sizeof (unsigned short); case TULONG: return sizeof (unsigned long); default: error(EXIT_FAILURE, 0, "datatype value of %d not recognized in " "gal_fits_datatype_size", datatype); } return 0; } void gal_fits_blank_to_value(void *array, int datatype, size_t size, void *value) { /* 'value' will only be read from one of these based on the datatype. Which the caller assigned. If there is any problem, it is their responsability, not this function's.*/ unsigned char *b, *bf, bv = *(uint8_t *) value; char *c, *cf, cv = *(char *) value; char **str, **strf, *strv = *(char **) value; short *s, *sf, sv = *(int16_t *) value; long *l, *lf, lv = *(int32_t *) value; LONGLONG *L, *Lf, Lv = *(int64_t *) value; float *f, *ff, fv = *(float *) value; double *d, *df, dv = *(double *) value; gsl_complex_float *cx, *cxf, cxv = *(gsl_complex_float *) value; gsl_complex *dcx, *dcxf, dcxv = *(gsl_complex *) value; int *in, *inf, inv = *(int *) value; unsigned int *ui, *uif, uiv = *(unsigned int *) value; unsigned short *us, *usf, usv = *(unsigned short *) value; unsigned long *ul, *ulf, ulv = *(unsigned long *) value; switch(datatype) { case TBIT: error(EXIT_FAILURE, 0, "Currently Gnuastro doesn't support TBIT " "datatype, please get in touch with us to implement it."); case TBYTE: bf=(b=array)+size; do if(*b==GAL_FITS_BYTE_BLANK) *b++=bv; while(bdatatype=datatype; newnode->keyname=keyname; newnode->value=value; newnode->comment=comment; newnode->unit=unit; newnode->kfree=kfree; /* Free pointers after using them. */ newnode->vfree=vfree; newnode->cfree=cfree; newnode->next=*list; *list=newnode; } void gal_fits_add_to_key_ll_end(struct gal_fits_key_ll **list, int datatype, char *keyname, int kfree, void *value, int vfree, char *comment, int cfree, char *unit) { struct gal_fits_key_ll *newnode, *tmp; /* Allocate space for the new node and fill it in. */ errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "linkedlist: new element in gal_fits_key_ll"); newnode->datatype=datatype; newnode->keyname=keyname; newnode->value=value; newnode->comment=comment; newnode->unit=unit; newnode->kfree=kfree; /* Free pointers after using them. */ newnode->vfree=vfree; newnode->cfree=cfree; if(*list) /* List is already full, add this node to the end */ { /* After this line, tmp points to the last node. */ tmp=*list; while(tmp->next!=NULL) tmp=tmp->next; tmp->next=newnode; newnode->next=NULL; } else /* List is empty */ { newnode->next=*list; *list=newnode; } } void gal_fits_file_name_in_keywords(char *keynamebase, char *filename, struct gal_fits_key_ll **list) { char *keyname, *value; size_t numkey=1, maxlength; size_t i, j, len=strlen(filename), thislen; /* When you give string arguments, CFITSIO puts them within two ''s, so the actual length available is two less. It seems this length also didn't include the null character, so, ultimately you have to take three from it.*/ maxlength=FLEN_VALUE-3; i=0; while(i0;--j) if(value[j]=='/') { value[j+1]='\0'; break; } if(j==0) error(EXIT_FAILURE, 0, "the filename `%sP has at least one " "span of %zu characters without a `/`. It cannot be " "written to the header of the output fits file", filename, maxlength); /* Convert the last useful character and save the file name.*/ gal_fits_add_to_key_ll_end(list, TSTRING, keyname, 1, value, 1, NULL, 0, NULL); i+=j+1; } } } /* Write the WCS and begin the part on this particular program's key words. */ void gal_fits_add_wcs_to_header(fitsfile *fptr, char *wcsheader, int nkeyrec) { size_t i; int h, status=0; char startblank[]=" / "; char *cp, *cpf, blankrec[80], titlerec[80]; /* Set the last element of the blank array. */ cpf=blankrec+79; *cpf='\0'; titlerec[79]='\0'; cp=blankrec; do *cp=' '; while(++cpvalue) { if( fits_update_key(fptr, tmp->datatype, tmp->keyname, tmp->value, tmp->comment, &status) ) gal_fits_io_error(status, NULL); } else { if(fits_update_key_null(fptr, tmp->keyname, tmp->comment, &status)) gal_fits_io_error(status, NULL); } if(tmp->unit && fits_write_key_unit(fptr, tmp->keyname, tmp->unit, &status) ) gal_fits_io_error(status, NULL); /* Free the value pointer if desired: */ if(tmp->kfree) free(tmp->keyname); if(tmp->vfree) free(tmp->value); if(tmp->cfree) free(tmp->comment); /* Keep the pointer to the next keyword and free the allocated space for this keyword.*/ ttmp=tmp->next; free(tmp); tmp=ttmp; } *keylist=NULL; } void gal_fits_write_keys_version(fitsfile *fptr, struct gal_fits_key_ll *headers, char *spack_string) { size_t i; int status=0; char *gitdescribe; char cfitsioversion[20]; char startblank[]=" / "; char *cp, *cpf, blankrec[80], titlerec[80]; /* Before WCSLIB 5.0, the wcslib_version function was not defined. Sometime in the future were everyone has moved to more recent versions of WCSLIB, we can remove this macro and its check in configure.ac.*/ #ifdef HAVE_WCSLIB_VERSION int wcslibvers[3]; char wcslibversion[20]; const char *wcslibversion_const; #endif /* Set the last element of the blank array. */ cpf=blankrec+79; *cpf='\0'; titlerec[79]='\0'; cp=blankrec; do *cp=' '; while(++cphstartwcs) { /* Mark the last character in the desired region. */ fullheader[hendwcs*(FLEN_CARD-1)]='\0'; /*******************************************************/ /****************************************************** printf("%s\n", fullheader); ******************************************************/ /*******************************************************/ /* Shift all the characters to the start of the string. */ if(hstartwcs) /* hstartwcs!=0 */ { to=fullheader; from=&fullheader[hstartwcs*(FLEN_CARD-1)-1]; while(*from++!='\0') *to++=*from; } nkeys=hendwcs-hstartwcs; /*******************************************************/ /****************************************************** printf("\n\n\n###############\n\n\n\n\n\n"); printf("%s\n", &fullheader[1*(FLEN_CARD-1)]); exit(0); ******************************************************/ /*******************************************************/ } /* WCSlib function */ status=wcspih(fullheader, nkeys, relax, ctrl, &nreject, nwcs, wcs); if(status) { fprintf(stderr, "\n##################\n" "WCSLIB Warning: wcspih ERROR %d: %s.\n" "##################\n", status, wcs_errmsg[status]); *wcs=NULL; *nwcs=0; } if (fits_free_memory(fullheader, &status) ) gal_fits_io_error(status, "problem in fitsarrayvv.c for freeing " "the memory used to keep all the headers"); /* Set the internal structure: */ status=wcsset(*wcs); if(status) { fprintf(stderr, "\n##################\n" "WCSLIB Warning: wcsset ERROR %d: %s.\n" "##################\n", status, wcs_errmsg[status]); *wcs=NULL; *nwcs=0; } /* Initialize the wcsprm struct if ((status = wcsset(*wcs))) error(EXIT_FAILURE, 0, "wcsset ERROR %d: %s.\n", status, wcs_errmsg[status]); */ } void gal_fits_read_wcs(char *filename, char *hdu, size_t hstartwcs, size_t hendwcs, int *nwcs, struct wcsprm **wcs) { int status=0; fitsfile *fptr; /* Check HDU for realistic conditions: */ gal_fits_read_hdu(filename, hdu, 0, &fptr); /* Read the WCS information: */ gal_fits_read_wcs_from_pointer(fptr, nwcs, wcs, hstartwcs, hendwcs); /* Close the FITS file: */ fits_close_file(fptr, &status); gal_fits_io_error(status, NULL); } /* Read a FITS image into an array corresponding to fitstype and also save the size of the array. If the image has any null pixels, their number is returned by this function. The value that is placed for those pixels is defined by the macros in fitsarrayvv.h and depends on the type of the data.*/ int gal_fits_hdu_to_array(char *filename, char *hdu, int *bitpix, void **array, size_t *s0, size_t *s1) { void *bitblank; fitsfile *fptr; long naxes[2], fpixel[]={1,1}; int status=0, anyblank=0, datatype; /* Check HDU for realistic conditions: */ gal_fits_read_hdu(filename, hdu, 0, &fptr); /* Get the bitpix and size of the image: */ gal_fits_img_bitpix_size(fptr, bitpix, naxes); *s0=naxes[1]; *s1=naxes[0]; /* Allocate space for the array. */ datatype=gal_fits_bitpix_to_datatype(*bitpix); bitblank=gal_fits_datatype_blank(datatype); *array=gal_fits_datatype_alloc(*s0 * *s1, datatype); /* Read the image into the allocated array: */ fits_read_pix(fptr, gal_fits_bitpix_to_datatype(*bitpix), fpixel, *s0 * *s1, bitblank, *array, &anyblank, &status); if(status) gal_fits_io_error(status, NULL); free(bitblank); /* Close the FITS file: */ fits_close_file(fptr, &status); gal_fits_io_error(status, NULL); /* Return the number of blank pixels: */ return anyblank; } /************************************************************* ****************** Array to FITS ****************** *************************************************************/ void gal_fits_array_to_file(char *filename, char *extname, int bitpix, void *array, size_t s0, size_t s1, int anyblank, struct wcsprm *wcs, struct gal_fits_key_ll *headers, char *spack_string) { int nkeyrec; void *blank; fitsfile *fptr; char *wcsheader; int status=0, datatype; long fpixel=1, naxis=2, nelements, naxes[]={s1,s0}; datatype=gal_fits_bitpix_to_datatype(bitpix); nelements=naxes[0]*naxes[1]; if(access(filename,F_OK) != -1 ) fits_open_file(&fptr,filename, READWRITE, &status); else fits_create_file(&fptr, filename, &status); fits_create_img(fptr, bitpix, naxis, naxes, &status); fits_write_img(fptr, datatype, fpixel, nelements, array, &status); if(anyblank) if(bitpix==BYTE_IMG || bitpix==SHORT_IMG || bitpix==LONG_IMG || bitpix==LONGLONG_IMG) { blank=gal_fits_datatype_blank( gal_fits_bitpix_to_datatype(bitpix) ); if(fits_write_key(fptr, datatype, "BLANK", blank, "Pixels with no data.", &status) ) gal_fits_io_error(status, "adding the BLANK keyword"); free(blank); } fits_write_key(fptr, TSTRING, "EXTNAME", extname, "", &status); gal_fits_io_error(status, NULL); if(wcs) { /* Convert the WCS information to text. */ status=wcshdo(WCSHDO_safe, wcs, &nkeyrec, &wcsheader); if(status) error(EXIT_FAILURE, 0, "wcshdo ERROR %d: %s", status, wcs_errmsg[status]); gal_fits_add_wcs_to_header(fptr, wcsheader, nkeyrec); } gal_fits_write_keys_version(fptr, headers, spack_string); fits_close_file(fptr, &status); gal_fits_io_error(status, NULL); } /* `atof' stands for "array to file". This is essentially the same as `gal_fits_array_to_file' except that the WCS structure's CRPIX values have changed. */ void gal_fits_atof_correct_wcs(char *filename, char *hdu, int bitpix, void *array, size_t s0, size_t s1, char *wcsheader, int wcsnkeyrec, double *crpix, char *spack_string) { fitsfile *fptr; int status=0, datatype; long fpixel=1, naxis=2, nelements, naxes[]={s1,s0}; datatype=gal_fits_bitpix_to_datatype(bitpix); nelements=naxes[0]*naxes[1]; if(access(filename,F_OK) != -1 ) fits_open_file(&fptr,filename, READWRITE, &status); else fits_create_file(&fptr, filename, &status); fits_create_img(fptr, bitpix, naxis, naxes, &status); fits_write_img(fptr, datatype, fpixel, nelements, array, &status); fits_write_key(fptr, TSTRING, "EXTNAME", hdu, "", &status); gal_fits_io_error(status, NULL); fits_delete_key(fptr, "COMMENT", &status); fits_delete_key(fptr, "COMMENT", &status); gal_fits_io_error(status, NULL); if(wcsheader) { gal_fits_add_wcs_to_header(fptr, wcsheader, wcsnkeyrec); if(crpix) { fits_update_key(fptr, TDOUBLE, "CRPIX1", &crpix[0], NULL, &status); fits_update_key(fptr, TDOUBLE, "CRPIX2", &crpix[1], NULL, &status); gal_fits_io_error(status, NULL); } } gal_fits_write_keys_version(fptr, NULL, spack_string); fits_close_file(fptr, &status); gal_fits_io_error(status, NULL); } /**************************************************************/ /********** Table ************/ /**************************************************************/ /* Get the size of a table HDU. CFITSIO doesn't use size_t, also we want to check status here.*/ void gal_fits_table_size(fitsfile *fitsptr, size_t *nrows, size_t *ncols) { long lnrows; int incols, status=0; /* Read the sizes and put them in. */ fits_get_num_rows(fitsptr, &lnrows, &status); fits_get_num_cols(fitsptr, &incols, &status); *ncols=incols; *nrows=lnrows; /* Report an error if any was issued. */ gal_fits_io_error(status, NULL); } int gal_fits_table_type(fitsfile *fptr) { int status=0; char value[FLEN_VALUE]; fits_read_key(fptr, TSTRING, "XTENSION", value, NULL, &status); if(status==0) { if(!strcmp(value, "TABLE ")) return ASCII_TBL; else if(!strcmp(value, "BINTABLE")) return BINARY_TBL; else error(EXIT_FAILURE, 0, "The `XTENSION' keyword of this FITS file " "doesn't have a standard value (`%s')", value); } else { if(status==KEY_NO_EXIST) error(EXIT_FAILURE, 0, "the `gal_fits_table_type' function was " "called on a FITS extension which is not a table. As part " "of a utility, this is bug, so please contact us at %s so " "we can fix it.", PACKAGE_BUGREPORT); else gal_fits_io_error(status, NULL); } error(EXIT_FAILURE, 0, "A bug! Please contact us at %s so we can fix it. " "for some reason, the control of `gal_fits_table_type' has reached " "the end of the function! This must not happen", PACKAGE_BUGREPORT); return -1; } /**************************************************************/ /********** Check prepare file ************/ /**************************************************************/ /* We have the name of the input file. But in most cases, the files that should be used (for example a mask image) are other extensions in the same file. So the user only has to give the HDU. The job of this function is to determine which is the case and set othername to the appropriate value. */ void gal_fits_file_or_ext_name(char *inputname, char *inhdu, int othernameset, char **othername, char *ohdu, int ohduset, char *type) { if(othernameset) { /* In some cases, for example a mask image, both the name and HDU are optional. So just to be safe, we will check this all the time. */ if(ohduset==0) error(EXIT_FAILURE, 0, "a %s image was specified (%s). However, " "no HDU is given for it. Please add a HDU. If you regularly " "use the same HDU as %s, you may consider adding it to " "the configuration file. For more information, please see " "the `Configuration files' section of the %s manual by " "running ` info gnuastro ' on the command-line", type, *othername, type, PACKAGE_NAME); if(strcmp(inputname, *othername)==0) { if(strcmp(ohdu, inhdu)==0) error(EXIT_FAILURE, 0, "the specified %s name and " "input image name (%s) are the same while the input " "image hdu name and mask hdu are also identical (%s)", type, inputname, inhdu); } } else if(ohduset && strcmp(ohdu, inhdu)) *othername=inputname; else *othername=NULL; } /* The user has specified an input file and a mask file. In the processing, all masked pixels will be converted to NaN pixels in the input image so we only have to deal with one array. Also since all processing is done on floating point arrays, the input is converted to floating point, irrespective of its input type. The original input bitpix will be stored so if you want to, you can return it back to the input type if you please. */ void gal_fits_file_to_float(char *inputname, char *maskname, char *inhdu, char *mhdu, float **img, int *inbitpix, int *anyblank, size_t *ins0, size_t *ins1) { void *array; int maskbitpix; float *mask, *f, *ff, *fp; size_t maskanyblank, s0, s1; /* Read the input array and convert it to float. */ *anyblank=gal_fits_hdu_to_array(inputname, inhdu, inbitpix, &array, ins0, ins1); if(*inbitpix==FLOAT_IMG) *img=array; else { gal_fits_change_type(array, *inbitpix, *ins0 * *ins1, *anyblank, (void **)img, FLOAT_IMG); free(array); } /* If a mask was specified, read it as a float image, then set all the corresponding pixels of the input image to NaN. */ if(maskname) { maskanyblank=gal_fits_hdu_to_array(maskname, mhdu, &maskbitpix, &array, &s0, &s1); if(maskbitpix==FLOAT_IMG || maskbitpix==DOUBLE_IMG) fprintf(stderr, "WARNING: the mask image (%s, hdu: %s) has a %s " "precision floating point data type (BITPIX=%d). The mask " "image is usually an integer type. Therefore this might " "be due to a mistake in the inputs and the results might " "not be what you intended. However, the program will not " "abort and continue working only with zero valued pixels " "in the given masked image.", maskname, mhdu, maskbitpix==FLOAT_IMG ? "single" : "double", maskbitpix); if(s0!=*ins0 || s1!=*ins1) error(EXIT_FAILURE, 0, "the input image %s (hdu: %s) has size: " "%zu x %zu. The mask image %s (hdu: %s) has size %zu x %zu. " "The two images have to have the same size", inputname, inhdu, *ins1, *ins0, maskname, mhdu, s1, s0); if(maskbitpix==FLOAT_IMG) mask=array; else { gal_fits_change_type(array, maskbitpix, *ins0 * *ins1, maskanyblank, (void **)(&mask), FLOAT_IMG); free(array); } ff=mask; fp=(f=*img)+s0*s1; do if(*ff++!=0.0f) {*f=NAN; ++(*anyblank);} while(++f Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include /* For mkdir permission flags. */ #include "checkset.h" #include "configfiles.h" /* Add the HOME environment variable to the given directory. */ char * gal_configfiles_add_home_dir(char *dir) { char *home; /* Get the home environment variable. */ home=getenv("HOME"); if(home==NULL) error(EXIT_FAILURE, 0, "the HOME environment variable " "is not defined"); /* Concatenate the two strings together: */ return gal_checkset_malloc_cat(home, dir); } void gal_configfiles_read_name_value(char *line, char *filename, size_t lineno, char **name, char **value) { int notyetfinished=1, inword=0, inquote=0; /* Initialize name and value: */ *name=NULL; *value=NULL; /* Go through the characters and set the values: */ do switch(*line) { case ' ': case '\t': case '\v': case '\n': case '\r': if(inword) /* Only considered in a word, not in a quote*/ { inword=0; *line='\0'; if(*value && inquote==0) notyetfinished=0; } break; case '#': notyetfinished=0; break; case '"': if(inword) error_at_line(EXIT_FAILURE, 0, filename, lineno, "Quotes have to be surrounded by whitespace " "characters (space, tab, new line, etc)."); if(inquote) { *line='\0'; inquote=0; notyetfinished=0; } else { if(*name==NULL) error_at_line(EXIT_FAILURE, 0, filename, lineno, "Parameter name should not start with " "double quotes (\")."); inquote=1; *value=line+1; } break; default: if(inword==0 && inquote==0) { if(*name==NULL) *name=line; else /* name is set, now assign *value. */ *value=line; inword=1; } break; } while(*(++line)!='\0' && notyetfinished); /* In the last line of the file, there is no new line to be converted to a '\0' character! So if value has been assigned, we are not in a quote and the line has finished, it means the given value has also finished. */ if(*line=='\0' && *value && inquote==0) notyetfinished=0; /* This was a blank line: */ if(*name==NULL && *value==NULL) return; /* Name or value were set but not yet finished. */ if(notyetfinished) error_at_line(EXIT_FAILURE, 0, filename, lineno, "line finished before parameter name and " "value could be read."); } FILE * gal_configfiles_write_local_config_stop(char *indir, char *filename, char *spack, char *spack_name, char **outfilename) { DIR *dp; FILE *fp; time_t rawtime; errno=0; time(&rawtime); /* Make sure the directory exists, if it doesn't, try to make it.*/ dp=opendir(indir); if(dp==NULL) /* The directory could not be opened. */ { if(errno==ENOENT) { errno=0; if(mkdir(indir, S_IRWXU)==-1) error(EXIT_FAILURE, errno, "%s: could not be created. Try " "running:\n\n mkdir -p %s\n\nto built it and run " "your previous command again", indir, indir); } else error(EXIT_FAILURE, errno, "%s", indir); } else { errno=0; if (closedir(dp)==-1) error(EXIT_FAILURE, errno, "%s", indir); } /* Make the local defaults file and put the top information in it. */ *outfilename=gal_checkset_malloc_cat(indir, filename); /* Check if the file opening was successful: */ errno=0; fp=fopen(*outfilename, "w"); if (fp==NULL) error(EXIT_FAILURE, errno, "%s", *outfilename); /* write the comments: */ fprintf(fp, "# Default parameters for %s (%s).\n" "# %s is part of GNU Astronomy Utitlies.\n" "# This file was created on %s#\n" "# Use the long option name of each parameter followed by\n" "# a value. The name and value should be separated by\n" "# at least one of the following characters:\n" "# space, `,`, `=` or `:`.\n#\n" "# Run `%s --help` or `info %s`\n" "# for more information.\n#\n" "# NOTE I: All counting is from zero, not one.\n" "# NOTE II: Lines starting with `#` are ignored.\n", spack_name, spack, spack_name, ctime(&rawtime), spack, spack); return fp; } void gal_configfiles_print_type(FILE *fp, int bitpix) { switch(bitpix) { case BYTE_IMG: fprintf(fp, CONF_SHOWFMT"%s\n", "type", "byte"); break; case SHORT_IMG: fprintf(fp, CONF_SHOWFMT"%s\n", "type", "short"); break; case LONG_IMG: fprintf(fp, CONF_SHOWFMT"%s\n", "type", "long"); break; case LONGLONG_IMG: fprintf(fp, CONF_SHOWFMT"%s\n", "type", "longlong"); break; case FLOAT_IMG: fprintf(fp, CONF_SHOWFMT"%s\n", "type", "float"); break; case DOUBLE_IMG: fprintf(fp, CONF_SHOWFMT"%s\n", "type", "double"); break; default: error(EXIT_FAILURE, 0, "a bug! the value of bitpix is not recognized " "in `gal_configfiles_print_type'. Please contact us at %s so " "we can address the problem.", PACKAGE_BUGREPORT); } } gnuastro-0.2.33-8a3b/lib/checkset.c0000644000175000017500000006025413001632540013621 00000000000000/********************************************************************* Functions to check and set command line argument values and files. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include "checkset.h" #define FIXEDFORFILE "The value of `%s` (given as %s)" #define FIXEDFOROPTION "The value of `--%s (-%c)` (given as %s)" #define NOTEMSG_NOTNUMBER "not readable as number" #define NOTEMSG_EQZEROORONE "should be ==0 or ==1" #define NOTEMSG_LEQZERO "should be >=0" #define NOTEMSG_LARGERZERO "should be >0" #define NOTEMSG_4OR8 "should be either 4 or 8" #define NOTEMSG_SMALLERONE "should be >=0 and <=1" #define CHECKFULLNUMBER if(*tailptr!='\0'){ \ if(filename) \ error_at_line(EXIT_FAILURE, 0, filename, lineno, \ FIXEDFORFILE" "NOTEMSG_NOTNUMBER, lo, optarg); \ else \ error(EXIT_FAILURE, 0, FIXEDFOROPTION" "NOTEMSG_NOTNUMBER, \ lo, so, optarg); \ } /**************************************************************** ************ Check and convert strings ***************** ****************************************************************/ /* See if a given string is a floating point number, if so, put it in the number.*/ int gal_checkset_str_is_double(char *string, double *out) { char *tailptr; double tmp=*out; *out=strtod(string, &tailptr); /* If the tail pointer (tailptr) is the string NULL character, then the string was a single double precision floating point number. However, if it is any other character, then put the initial value of out back inside of it and return 0. */ if(*tailptr=='\0') return 1; *out=tmp; return 0; } /**************************************************************** ***************** Check the numbers ******************** ****************************************************************/ void gal_checkset_int_zero_or_one(char *optarg, int *var, char *lo, char so, char *spack, char *filename, size_t lineno) { long tmp; char *tailptr; *var=tmp=strtol(optarg, &tailptr, 0); CHECKFULLNUMBER; if(tmp!=0 && tmp!=1) { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, FIXEDFORFILE" "NOTEMSG_EQZEROORONE, lo, optarg); else error(EXIT_FAILURE, 0, FIXEDFOROPTION" "NOTEMSG_EQZEROORONE, lo, so, optarg); } } void gal_checkset_int_4_or_8(char *optarg, int *var, char *lo, char so, char *spack, char *filename, size_t lineno) { long tmp; char *tailptr; *var=tmp=strtol(optarg, &tailptr, 0); CHECKFULLNUMBER; if(tmp!=4 && tmp!=8) { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, FIXEDFORFILE" "NOTEMSG_EQZEROORONE, lo, optarg); else error(EXIT_FAILURE, 0, FIXEDFOROPTION" "NOTEMSG_EQZEROORONE, lo, so, optarg); } } void gal_checkset_int_el_zero(char *optarg, int *var, char *lo, char so, char *spack, char *filename, size_t lineno) { long tmp; char *tailptr; *var=tmp=strtol(optarg, &tailptr, 0); CHECKFULLNUMBER; if(tmp<0) { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, FIXEDFORFILE" "NOTEMSG_LEQZERO, lo, optarg); else error(EXIT_FAILURE, 0, FIXEDFOROPTION" "NOTEMSG_LEQZERO, lo, so, optarg); } } void gal_checkset_int_l_zero(char *optarg, int *var, char *lo, char so, char *spack, char *filename, size_t lineno) { long tmp; char *tailptr; *var=tmp=strtol(optarg, &tailptr, 0); CHECKFULLNUMBER; if(tmp<=0) { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, FIXEDFORFILE" "NOTEMSG_LARGERZERO, lo, optarg); else error(EXIT_FAILURE, 0, FIXEDFOROPTION" "NOTEMSG_LARGERZERO, lo, so, optarg); } } void gal_checkset_int_smaller_equal_to(char *optarg, int *var, char *lo, char so, char *spack, char *filename, size_t lineno, long maxvalue) { long tmp; char *tailptr; *var=tmp=strtol(optarg, &tailptr, 0); CHECKFULLNUMBER; if(tmp>maxvalue) { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, FIXEDFORFILE" "NOTEMSG_4OR8, lo, optarg); else error(EXIT_FAILURE, 0, FIXEDFOROPTION" "NOTEMSG_4OR8, lo, so, optarg); } } void gal_checkset_long_el_zero(char *optarg, long *var, char *lo, char so, char *spack, char *filename, size_t lineno) { long tmp; char *tailptr; *var=tmp=strtol(optarg, &tailptr, 0); CHECKFULLNUMBER; if(tmp<0) { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, FIXEDFORFILE" "NOTEMSG_LEQZERO, lo, optarg); else error(EXIT_FAILURE, 0, FIXEDFOROPTION" "NOTEMSG_LEQZERO, lo, so, optarg); } } void gal_checkset_any_long(char *optarg, long *var, char *lo, char so, char *spack, char *filename, size_t lineno) { char *tailptr; *var=strtol(optarg, &tailptr, 0); CHECKFULLNUMBER; } /* size_t is always >=0. But if the user gives a negative value, it will become an extremely large number (because size_t is unsigned). So we read the user's value in long, which accepts negative values, then we check that value before placing it in the size_t pointer.*/ void gal_checkset_sizet_el_zero(char *optarg, size_t *var, char *lo, char so, char* spack, char *filename, size_t lineno) { long tmp; char *tailptr; *var=tmp=strtol(optarg, &tailptr, 0); CHECKFULLNUMBER; if(tmp<0) { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, FIXEDFORFILE" "NOTEMSG_LEQZERO, lo, optarg); else error(EXIT_FAILURE, 0, FIXEDFOROPTION" "NOTEMSG_LEQZERO, lo, so, optarg); } } /* See explanation for gal_checkset_sizet_l_zero above. */ void gal_checkset_sizet_l_zero(char *optarg, size_t *var, char *lo, char so, char* spack, char *filename, size_t lineno) { long tmp; char *tailptr; *var=tmp=strtol(optarg, &tailptr, 0); CHECKFULLNUMBER; if(tmp<=0) { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, FIXEDFORFILE" "NOTEMSG_LARGERZERO, lo, optarg); else error(EXIT_FAILURE, 0, FIXEDFOROPTION" "NOTEMSG_LARGERZERO, lo, so, optarg); } } /* Positive and odd size_t. */ void gal_checkset_sizet_p_odd(char *optarg, size_t *var, char *lo, char so, char* spack, char *filename, size_t lineno) { long tmp; char *tailptr; *var=tmp=strtol(optarg, &tailptr, 0); CHECKFULLNUMBER; if(tmp<0 || tmp%2==0) { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, FIXEDFORFILE" should be >0 and odd.", lo, optarg); else error(EXIT_FAILURE, 0, FIXEDFOROPTION" should be >0 and odd", lo, so, optarg); } } void gal_checkset_float_l_0(char *optarg, float *var, char *lo, char so, char* spack, char *filename, size_t lineno) { float tmp; char *tailptr; *var=tmp=strtof(optarg, &tailptr); CHECKFULLNUMBER; if(tmp<=0) { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, FIXEDFORFILE" "NOTEMSG_LARGERZERO, lo, optarg); else error(EXIT_FAILURE, 0, FIXEDFOROPTION" "NOTEMSG_LARGERZERO, lo, so, optarg); } } void gal_checkset_float_l_0_s_1(char *optarg, float *var, char *lo, char so, char* spack, char *filename, size_t lineno) { float tmp; char *tailptr; *var=tmp=strtof(optarg, &tailptr); CHECKFULLNUMBER; if(tmp>1.0f || tmp<0) { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, FIXEDFORFILE" "NOTEMSG_SMALLERONE, lo, optarg); else error(EXIT_FAILURE, 0, FIXEDFOROPTION" "NOTEMSG_SMALLERONE, lo, so, optarg); } } void gal_checkset_any_float(char *optarg, float *var, char *lo, char so, char *spack, char *filename, size_t lineno) { char *tailptr; *var=strtof(optarg, &tailptr); CHECKFULLNUMBER; } void gal_checkset_double_l_0(char *optarg, double *var, char *lo, char so, char* spack, char *filename, size_t lineno) { double tmp; char *tailptr; *var=tmp=strtod(optarg, &tailptr); CHECKFULLNUMBER; if(tmp<=0) { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, FIXEDFORFILE" "NOTEMSG_LARGERZERO, lo, optarg); else error(EXIT_FAILURE, 0, FIXEDFOROPTION" "NOTEMSG_LARGERZERO, lo, so, optarg); } } void gal_checkset_double_el_0(char *optarg, double *var, char *lo, char so, char* spack, char *filename, size_t lineno) { double tmp; char *tailptr; *var=tmp=strtod(optarg, &tailptr); CHECKFULLNUMBER; if(tmp<0) { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, FIXEDFORFILE" "NOTEMSG_LARGERZERO, lo, optarg); else error(EXIT_FAILURE, 0, FIXEDFOROPTION" "NOTEMSG_LARGERZERO, lo, so, optarg); } } void gal_checkset_double_l_value(char *optarg, double *var, char *lo, char so, char* spack, double value, char *filename, size_t lineno) { float tmp; char *tailptr; *var=tmp=strtof(optarg, &tailptr); CHECKFULLNUMBER; if(tmp<=value) { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, FIXEDFORFILE" should be > %.4f", lo, optarg, value); else error(EXIT_FAILURE, 0, FIXEDFOROPTION" should be > %.4f", lo, so, optarg, value); } } void gal_checkset_any_double(char *optarg, double *var, char *lo, char so, char *spack, char *filename, size_t lineno) { char *tailptr; *var=strtod(optarg, &tailptr); CHECKFULLNUMBER; } /**************************************************************/ /********** Check fixed strings ************/ /**************************************************************/ /* Check if the value to the `--type' option is recognized, if so set the integer value. */ void gal_checkset_known_types(char *optarg, int *bitpix, char *filename, size_t lineno) { /* First check if the value is one of the accepted types. */ if (strcmp(optarg, "byte")==0) *bitpix=BYTE_IMG; else if(strcmp(optarg, "short")==0) *bitpix=SHORT_IMG; else if(strcmp(optarg, "long")==0) *bitpix=LONG_IMG; else if(strcmp(optarg, "longlong")==0) *bitpix=LONGLONG_IMG; else if(strcmp(optarg, "float")==0) *bitpix=FLOAT_IMG; else if(strcmp(optarg, "double")==0) *bitpix=DOUBLE_IMG; else { if(filename) error_at_line(EXIT_FAILURE, 0, filename, lineno, "given value of " "the `type' option (`%s') is not recognized. It must " "be `byte', `short', `long', `longlong', `float', or " "`double'.", optarg); else error(EXIT_FAILURE, 0, "given value of the `--type' (`-T') option " "(`%s') is not recognized. It must be `byte', `short', `long' " "`longlong', `float', or `double'.", optarg); } } /**************************************************************/ /********** My String functions: ************/ /**************************************************************/ int gal_checkset_string_has_space(char *in) { do switch(*in) { case ' ': case '\t': case '\v': return 1; } while(*(++in)!='\0'); return 0; } char * gal_checkset_malloc_cat(char *inname, char *toappend) { char *out; size_t inl, apl; inl=strlen(inname); apl=strlen(toappend); errno=0; out=malloc(inl+apl+1); if(out==NULL) error(EXIT_FAILURE, errno, "allocating %zu bytes in gal_checkset_malloc_cat", inl+apl+1); strcpy(out, inname); strcat(out, toappend); return out; } /* Copy the input string to the output (and also allocate the output. */ void gal_checkset_allocate_copy(char *arg, char **copy) { /* Allocate the necessary space: */ errno=0; *copy=malloc(strlen(arg)+1); if(*copy==NULL) error(EXIT_FAILURE, errno, "%zu bytes to copy %s", strlen(arg)+1, arg); strcpy(*copy, arg); } /* This function is mainly for reading in the arguments (from the command line or configuration files) that need to be copied. The set argument is for making sure that it has not already been set before, see the main.h files of any program. */ void gal_checkset_allocate_copy_set(char *arg, char **copy, int *set) { /* Incase *set==1, then you shouldn't do anything, just return. */ if(*set) return; /* The variable was not copied, copy it: */ errno=0; *copy=malloc(strlen(arg)+1); if(*copy==NULL) error(EXIT_FAILURE, errno, "%zu bytes to copy %s", strlen(arg)+1, arg); strcpy(*copy, arg); *set=1; } /**************************************************************/ /********** Set file names and check if they exist ************/ /**************************************************************/ /* Check if a file exists and report if it doesn't: */ void gal_checkset_check_file(char *filename) { FILE *tmpfile; errno=0; tmpfile = fopen(filename, "r"); if(tmpfile) /* The file opened. */ { if(fclose(tmpfile)==EOF) error(EXIT_FAILURE, errno, "%s", filename); } else error(EXIT_FAILURE, errno, "%s", filename); } /* Similar to `gal_checkset_check_file', but will report the result instead of doing it quietly. */ int gal_checkset_check_file_report(char *filename) { FILE *tmpfile; errno=0; tmpfile = fopen(filename, "r"); if(tmpfile) /* The file opened. */ { if(fclose(tmpfile)==EOF) error(EXIT_FAILURE, errno, "%s", filename); return 1; } else return 0; } /* Check if a file exists. If so, remove it. */ void gal_checkset_check_remove_file(char *filename, int dontdelete) { FILE *tmpfile; /* We want to make sure that we can open and write to this file. But the user might have asked to not delete the file, so the contents should not be changed. Therefore we have to open it with `r+`. */ errno=0; tmpfile=fopen(filename, "r+"); if (tmpfile) /* The file opened. */ { /* Close the file and make sure that it should be deleted. */ errno=0; if(fclose(tmpfile)) error(EXIT_FAILURE, errno, "%s", filename); if(dontdelete) error(EXIT_FAILURE, 0, "%s already exists and you have " "asked to not remove it with the `--dontdelete` " "(`-D`) option", filename); /* Delete the file: */ errno=0; if(unlink(filename)) error(EXIT_FAILURE, errno, "%s", filename); } /* If the file doesn't exist, there is no problem, we wanted to remove it any way! Any other kind of error should not be tolerated! */ else if(errno!=ENOENT) error(EXIT_FAILURE, errno, "%s", filename); } /* Check output file name: If a file exists or can exist and can be written to, this function will return 1. If not (for example it is a directory) it will return 0. Finally, if it exists but cannot be deleted, report an error and abort. */ int gal_checkset_dir_0_file_1(char *name, int dontdelete) { FILE *tmpfile; struct stat nameinfo; if(name==NULL) error(EXIT_FAILURE, 0, "a bug! The input to the " "gal_checkset_dir_0_file_1 function in checkset.c should not " "be NULL. Please contact us at "PACKAGE_BUGREPORT" so we can " "see what went wrong and fix it in future updates"); errno=0; if(stat(name, &nameinfo)!=0) { if(errno==ENOENT) /* ENOENT: No such file or directory. */ {/* Make the file temporarily and see if everything is ok. */ errno=0; tmpfile=fopen(name, "w"); if (tmpfile) { fprintf(tmpfile, "Only to test write access."); errno=0; if(fclose(tmpfile)) error(EXIT_FAILURE, errno, "%s", name); errno=0; if(unlink(name)) error(EXIT_FAILURE, errno, "%s", name); } else error(EXIT_FAILURE, errno, "%s", name); return 1; /* It is a file name, GOOD */ } else /* Some strange condition, ABORT */ error(EXIT_FAILURE, errno, "%s", name); } if(S_ISDIR(nameinfo.st_mode)) /* It is a directory, BAD */ return 0; else if (S_ISREG(nameinfo.st_mode)) /* It is a file, GOOD. */ { gal_checkset_check_remove_file(name, dontdelete); return 1; } else /* Not a file or a dir, ABORT */ error(EXIT_FAILURE, 0, "%s not a file or a directory", name); error(EXIT_FAILURE, 0, "a bug! In gal_checkset_dir_0_file_1, (in " "checkset.c). The process should not reach the end of the " "function! Please contact us at "PACKAGE_BUGREPORT" so we can " "see what went wrong and fix it in future updates"); return 0; } /* Allocate space and write the output name (outname) based on a given input name (inname). The suffix of the input name (if present) will be removed and the given suffix will be put in the end. */ void gal_checkset_automatic_output(char *inname, char *suffix, int removedirinfo, int dontdelete, char **outname) { char *out; size_t i, l, offset=0; /* Merge the contents of the input name and suffix name (while also allocating the necessary space).*/ out=gal_checkset_malloc_cat(inname, suffix); /* If there is actually a suffix, replace it with the (possibly) existing suffix. */ if(suffix[0]!='\0') { /* Start from the end of the input array*/ l=strlen(inname); for(i=l-1;i!=0;--i) { /* We don't want to touch anything before a `/' (directory names). We are only concerned with file names here. */ if(out[i]=='/') { /* When `/' is the last input character, then the input is clearly not a filename, but a directory name. In this case, adding a suffix is meaningless (a suffix belongs to a filename for Gnuastro's tools). So close the string after the `/' and leave the loop. However, if the `/' isn't the last input name charector, there is probably a filename (without a "." suffix), so break from the loop. No further action is required, since we initially allocated the necessary space and concatenated the input and suffix arrays. */ if(i==l-1) out[i+1]='\0'; break; } else if(out[i]=='.') { out[i]='\0'; strcat(out, suffix); break; } } } /* If it is desired to remove the directory information from the name, do it here. Some unused space will remain after removing the directory information, but that can be ignored, since it can't be too much. */ if(removedirinfo) { l=strlen(out); for(i=l;i!=0;--i) /* Find the last forward slash. */ if(out[i]=='/') {offset=i+1; break;} if(offset) for(i=offset;i<=l;++i) /* <= because we want to shift the */ out[i-offset]=out[i]; /* '\0' character in the string too. */ } /* Remove the created filename if it already exits. */ gal_checkset_check_remove_file(out, dontdelete); /* Free the outname if it was already allocated before. */ free(*outname); *outname=out; } /* Given a filename, this function will separate its directory name part. */ char * gal_checkset_dir_part(char *input) { char *out; size_t i, l; /* Find the first slash. */ l=strlen(input); for(i=l;i!=0;--i) if(input[i]=='/') break; /* If there was no slash, then the current directory should be given: */ if(i==0) { errno=0; out=malloc(3*sizeof *out); if(out==NULL) error(EXIT_FAILURE, errno, "%zu bytes for current directory " "gal_checkset_dir_part", 3*sizeof *out); strcpy(out, "./"); } else { errno=0; out=malloc((l+1)*sizeof *out); if(out==NULL) error(EXIT_FAILURE, errno, "%zu bytes for gal_checkset_dir_part", (l+1)*sizeof *out); strcpy(out, input); out[i+1]='\0'; } return out; } /* Given a file name, keep the non-directory part. Note that if there is no forward slash in the input name, the full input name is considered to be the notdir output.*/ char * gal_checkset_not_dir_part(char *input) { size_t i, l; char *out, *tmp=input; /* Find the first `/' to identify the directory */ l=strlen(input); for(i=l;i!=0;--i) if(input[i]=='/') { tmp=&input[i+1]; break; } /* Get the length of the notdir name: */ l=strlen(tmp); errno=0; out=malloc((l+1)*sizeof *out); if(out==NULL) error(EXIT_FAILURE, errno, "%zu bytes for notdir", (l+1)*sizeof *out); strcpy(out, tmp); return out; } /* Check if dirname is actually a real directory and that we can actually write inside of it. To insure all conditions an actual file will be made */ void gal_checkset_check_dir_write_add_slash(char **dirname) { int file_d; char *tmpname, *indir=*dirname/*, buf[]="A test"*/; /* Set the template for the temporary file: */ if(indir[strlen(indir)-1]=='/') tmpname=gal_checkset_malloc_cat(indir, "gnuastroXXXXXX"); else tmpname=gal_checkset_malloc_cat(indir, "/gnuastroXXXXXX"); /* Make a temporary file name and try openning it. */ errno=0; file_d=mkstemp(tmpname); if(file_d==-1) error(EXIT_FAILURE, errno, "cannot write output in the directory %s", indir); /* errno=0; printf("\n\n%s\n\n", tmpname); if( write(file_d, buf, strlen(buf)) == -1 ) error(EXIT_FAILURE, errno, "%s: writing to this temporary file to " "check the given `%s` directory", tmpname, indir); */ errno=0; if( close(file_d) == -1 ) error(EXIT_FAILURE, errno, "%s: Closing this temporary file to check " "the given `%s` directory", tmpname, indir); /* Delete the temporary file: */ errno=0; if(unlink(tmpname)==-1) error(EXIT_FAILURE, errno, "%s: removing this temporary file made " "to check the given `%s directory`", tmpname, indir); /* Remove the extra characters that were added for the random name. */ tmpname[strlen(tmpname)-14]='\0'; free(*dirname); *dirname=tmpname; } gnuastro-0.2.33-8a3b/lib/box.c0000644000175000017500000002114212750745735012636 00000000000000/********************************************************************* overlap -- Find the overlap of a region and an image. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include /* IMPORTANT NOTE: All the axises are based on the FITS standard, not C. */ /* Any ellipse can be enclosed into a rectangular box. The purpose of this function is to give the height and width of that box. The logic behind it is this: All the points on the circumference of an ellipse that is aligned on the x axis can be written as: (acos(t),bsin(t)) where 0=0.5) ++lxc; lyc=yc; if (fabs(modf(yc, &intpart))>=0.5) ++lyc; /* Set the initial values for the actual image: */ fpixel[0]=lxc-width[0]/2; fpixel[1]=lyc-width[1]/2; lpixel[0]=lxc+width[0]/2; lpixel[1]=lyc+width[1]/2; /* printf("\n\nCenter is on: %ld, %ld\n", lxc, lyc); printf("Starting and ending pixels: (%ld, %ld) -- (%ld, %ld)\n\n\n", fpixel[0], fpixel[1], lpixel[0], lpixel[1]); */ } /* Problem to solve: We have set the first and last pixels in an input image (fpixel_i[2] and lpixel_i[2]). But those first and last pixels don't necessarily have to lie within the image, they can be outside of it or patially overlap with it. So the job of this function is to correct for such situations and find the starting and ending points of any overlap. It is assumed that your output (overlap) image's first pixel lies right ontop of the fpixel_i[0] in the input image. But since fpixel_i might be outside of the image, in this function we find the fpixel_o[2] and lpixel_o[2] in the overlap image coordinates that overlap with the input image. So the values of all four points might change after this function. Before: ======= fpixel_o and lpixel_o are not shown. fpixel_o and lpixel_o point to the same place as fpixel_i and lpixel_i, But in the coordinates of the overlap image. -----------------lpixel_i | overlap | | image | | | ----------------------|------ | | | | | | fpixel_i ----------------- | | | | | | | Input image | ----------------------------- After ===== ----------------- | overlap | | image | | | ----------------------|------lpixel_i | | | | | | fpixel_i ----------------- | | | | | | | Input image | ----------------------------- So in short the arrays we are dealing with here are: fpixel_i: Coordinates of the first pixel in input image. lpixel_i: Coordinates of the last pixel in input image. fpixel_o: Coordinates of the first pixel in overlap image. lpixel_o: Coordinates of the last pixel in overlap image. NOTES: ====== - lpixel is the last pixel in the image (not outside of it). - The coordinates are in the FITS format. Return value: ============= 1: There is an overlap 0: There is no overlap */ int gal_box_overlap(long *naxes, long *fpixel_i, long *lpixel_i, long *fpixel_o, long *lpixel_o) { long width[2]; /* In case you want to see how things are going: printf("\n\nImage size: [%ld, %ld]\n", naxes[0], naxes[1]); printf("fpixel_i -- lpixel_i: (%ld, %ld) -- (%ld, %ld)\n\n", fpixel_i[0], fpixel_i[1], lpixel_i[0], lpixel_i[1]); */ width[0]=lpixel_i[0]-fpixel_i[0]+1; width[1]=lpixel_i[1]-fpixel_i[1]+1; /* Set the initial values for the cropped array: */ fpixel_o[0]=1; fpixel_o[1]=1; lpixel_o[0]=width[0]; lpixel_o[1]=width[1]; /* Check the four corners to see if they should be adjusted: To understand the first, look at this, suppose | separates pixels and the * shows where the image actually begins. |-2|-1| 0* 1| 2| 3| 4| (survey image) *1 | 2| 3| 4| 5| 6| 7| (crop image) So when fpixel_i is negative, e.g., fpixel_i=-2, then the index of the pixel in the cropped image we want to begin with, that corresponds to 1 in the survey image is: fpixel_o= 4 = 2 + -1*fpixel_i.*/ if(fpixel_i[0]<1) { fpixel_o[0]=-1*fpixel_i[0]+2; fpixel_i[0]=1; } if(fpixel_i[1]<1) { fpixel_o[1]=-1*fpixel_i[1]+2; fpixel_i[1]=1; } /*The same principle applies to the end of an image. Take "s" is the maximum size along a specific axis in the survey image and "c" is the size along the same axis on the cropped image. Assume the the cropped region's last pixel in that axis will be 2 pixels larger than s: |s-1| s* s+1| s+2| (survey image) |c-3| c-2| c-1| c* (crop image) So you see that if the outer pixel is n pixels away then in the cropped image we should only fill upto c-n.*/ if (lpixel_i[0]>naxes[0]) { lpixel_o[0]=width[0]-(lpixel_i[0]-naxes[0]); lpixel_i[0]=naxes[0]; } if (lpixel_i[1]>naxes[1]) { lpixel_o[1]=width[1]-(lpixel_i[1]-naxes[1]); lpixel_i[1]=naxes[1]; } /* In case you wish to see the results. printf("\nAfter correction:\n"); printf("Input image: (%ld, %ld) -- (%ld, %ld)\n", fpixel_i[0], fpixel_i[1], lpixel_i[0], lpixel_i[1]); printf("output image:(%ld, %ld) -- (%ld, %ld)\n\n\n", fpixel_o[0], fpixel_o[1], lpixel_o[0], lpixel_o[1]); */ if(fpixel_i[0]>naxes[0] || fpixel_i[1]>naxes[1] || lpixel_i[0]<1 || lpixel_i[1]<1) return 0; else return 1; } gnuastro-0.2.33-8a3b/lib/array.c0000644000175000017500000001761013001632540013144 00000000000000/********************************************************************* Functions to manipulate arrays. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /********************************************************************* ********************** Initialize ********************** *********************************************************************/ void gal_array_uchar_init_on_region(unsigned char *in, const unsigned char v, size_t start, size_t s0, size_t s1, size_t is1) { size_t r; unsigned char *p, *fp; for(r=0;r&2; \ exit 1;; \ esac; \ has_opt=no; \ sane_makeflags=$$MAKEFLAGS; \ if $(am__is_gnu_make); then \ sane_makeflags=$$MFLAGS; \ else \ case $$MAKEFLAGS in \ *\\[\ \ ]*) \ bs=\\; \ sane_makeflags=`printf '%s\n' "$$MAKEFLAGS" \ | sed "s/$$bs$$bs[$$bs $$bs ]*//g"`;; \ esac; \ fi; \ skip_next=no; \ strip_trailopt () \ { \ flg=`printf '%s\n' "$$flg" | sed "s/$$1.*$$//"`; \ }; \ for flg in $$sane_makeflags; do \ test $$skip_next = yes && { skip_next=no; continue; }; \ case 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GNULIB_BTOWC = @GNULIB_BTOWC@ GNULIB_CALLOC_POSIX = @GNULIB_CALLOC_POSIX@ GNULIB_CANONICALIZE_FILE_NAME = @GNULIB_CANONICALIZE_FILE_NAME@ GNULIB_CBRT = @GNULIB_CBRT@ GNULIB_CBRTF = @GNULIB_CBRTF@ GNULIB_CBRTL = @GNULIB_CBRTL@ GNULIB_CEIL = @GNULIB_CEIL@ GNULIB_CEILF = @GNULIB_CEILF@ GNULIB_CEILL = @GNULIB_CEILL@ GNULIB_CHDIR = @GNULIB_CHDIR@ GNULIB_CHOWN = @GNULIB_CHOWN@ GNULIB_CLOSE = @GNULIB_CLOSE@ GNULIB_COPYSIGN = @GNULIB_COPYSIGN@ GNULIB_COPYSIGNF = @GNULIB_COPYSIGNF@ GNULIB_COPYSIGNL = @GNULIB_COPYSIGNL@ GNULIB_COSF = @GNULIB_COSF@ GNULIB_COSHF = @GNULIB_COSHF@ GNULIB_COSL = @GNULIB_COSL@ GNULIB_DPRINTF = @GNULIB_DPRINTF@ GNULIB_DUP = @GNULIB_DUP@ GNULIB_DUP2 = @GNULIB_DUP2@ GNULIB_DUP3 = @GNULIB_DUP3@ GNULIB_DUPLOCALE = @GNULIB_DUPLOCALE@ GNULIB_ENVIRON = @GNULIB_ENVIRON@ GNULIB_EUIDACCESS = @GNULIB_EUIDACCESS@ GNULIB_EXP2 = @GNULIB_EXP2@ GNULIB_EXP2F = @GNULIB_EXP2F@ GNULIB_EXP2L = @GNULIB_EXP2L@ GNULIB_EXPF = @GNULIB_EXPF@ GNULIB_EXPL = @GNULIB_EXPL@ GNULIB_EXPM1 = @GNULIB_EXPM1@ GNULIB_EXPM1F = @GNULIB_EXPM1F@ GNULIB_EXPM1L = @GNULIB_EXPM1L@ GNULIB_FABSF = @GNULIB_FABSF@ GNULIB_FABSL = @GNULIB_FABSL@ GNULIB_FACCESSAT = @GNULIB_FACCESSAT@ GNULIB_FCHDIR = @GNULIB_FCHDIR@ GNULIB_FCHMODAT = @GNULIB_FCHMODAT@ GNULIB_FCHOWNAT = @GNULIB_FCHOWNAT@ GNULIB_FCLOSE = @GNULIB_FCLOSE@ GNULIB_FCNTL = @GNULIB_FCNTL@ GNULIB_FDATASYNC = @GNULIB_FDATASYNC@ GNULIB_FDOPEN = @GNULIB_FDOPEN@ GNULIB_FFLUSH = @GNULIB_FFLUSH@ GNULIB_FFS = @GNULIB_FFS@ GNULIB_FFSL = @GNULIB_FFSL@ GNULIB_FFSLL = @GNULIB_FFSLL@ GNULIB_FGETC = @GNULIB_FGETC@ GNULIB_FGETS = @GNULIB_FGETS@ GNULIB_FLOOR = @GNULIB_FLOOR@ GNULIB_FLOORF = @GNULIB_FLOORF@ GNULIB_FLOORL = @GNULIB_FLOORL@ GNULIB_FMA = @GNULIB_FMA@ GNULIB_FMAF = @GNULIB_FMAF@ GNULIB_FMAL = @GNULIB_FMAL@ GNULIB_FMOD = @GNULIB_FMOD@ GNULIB_FMODF = @GNULIB_FMODF@ GNULIB_FMODL = @GNULIB_FMODL@ GNULIB_FOPEN = @GNULIB_FOPEN@ GNULIB_FPRINTF = @GNULIB_FPRINTF@ GNULIB_FPRINTF_POSIX = @GNULIB_FPRINTF_POSIX@ GNULIB_FPURGE = @GNULIB_FPURGE@ GNULIB_FPUTC = @GNULIB_FPUTC@ GNULIB_FPUTS = @GNULIB_FPUTS@ GNULIB_FREAD = @GNULIB_FREAD@ GNULIB_FREOPEN = @GNULIB_FREOPEN@ GNULIB_FREXP = @GNULIB_FREXP@ GNULIB_FREXPF = @GNULIB_FREXPF@ GNULIB_FREXPL = @GNULIB_FREXPL@ GNULIB_FSCANF = @GNULIB_FSCANF@ GNULIB_FSEEK = @GNULIB_FSEEK@ GNULIB_FSEEKO = @GNULIB_FSEEKO@ GNULIB_FSTAT = @GNULIB_FSTAT@ GNULIB_FSTATAT = @GNULIB_FSTATAT@ GNULIB_FSYNC = @GNULIB_FSYNC@ GNULIB_FTELL = @GNULIB_FTELL@ GNULIB_FTELLO = @GNULIB_FTELLO@ GNULIB_FTRUNCATE = @GNULIB_FTRUNCATE@ GNULIB_FUTIMENS = @GNULIB_FUTIMENS@ GNULIB_FWRITE = @GNULIB_FWRITE@ GNULIB_GETC = @GNULIB_GETC@ GNULIB_GETCHAR = @GNULIB_GETCHAR@ GNULIB_GETCWD = @GNULIB_GETCWD@ GNULIB_GETDELIM = @GNULIB_GETDELIM@ GNULIB_GETDOMAINNAME = @GNULIB_GETDOMAINNAME@ GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = 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without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. NOTE: $(top_srcdir)/bootstrapped/lib is only necessary ## for internally compiled utilities and libraries. It must not be included ## during the tests since the bootstrapped libraries are not installed. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib # Define the main compiled library file and its Libtool version. lib_LTLIBRARIES = libgnuastro.la libgnuastro_la_LDFLAGS = -version-info $(GAL_LT_VERSION) # Specify the library .c files libgnuastro_la_SOURCES = array.c box.c checkset.c configfiles.c fits.c \ git.c linkedlist.c mesh.c mode.c polygon.c qsort.c spatialconvolve.c \ statistics.c threads.c timing.c txtarray.c wcs.c # Installed headers, note that we are not blindly including all `.h' files # in the $(headersdir) directory. Some of the header files don't need to be # installed. pkginclude_HEADERS = gnuastro/gnuastro.h $(headersdir)/array.h \ $(headersdir)/box.h $(headersdir)/fits.h $(headersdir)/git.h \ $(headersdir)/linkedlist.h $(headersdir)/mesh.h $(headersdir)/polygon.h \ $(headersdir)/qsort.h $(headersdir)/spatialconvolve.h \ $(headersdir)/statistics.h $(headersdir)/threads.h $(headersdir)/wcs.h \ $(headersdir)/txtarray.h # Files to distribute in the tarball. These are internal headers and don't # need to be installed. Headers are only mentioned within the source files, # and if they are not explicitly mentioned somewhere in the Makefile, they # will not distributed, so we need to explicitly tell Automake to # distribute them here. headersdir=$(top_srcdir)/lib/gnuastro EXTRA_DIST = gnuastro.pc.in gnuastro.h.in checkset.h commonargs.h \ commonparams.h configfiles.h fixedstringmacros.h mode.h neighbors.h \ timing.h $(headersdir)/README # Definitions for Gnuastro's the pkg-config file (inspired from GSL's # Makefile.am) pkgconfig_DATA = gnuastro.pc pkgconfigdir = $(libdir)/pkgconfig CLEANFILES = gnuastro.pc gnuastro/gnuastro.h # Build Gnuastro's pkg-config file and `gnuastro.h' based on the # information in the Makefile after the Makefile has been built. gnuastro/gnuastro.h: Makefile gnuastro.h.in rm -f $@ $@.tmp $(MKDIR_P) gnuastro $(SED) -e 's|@VERSION[@]|$(VERSION)|g' \ -e 's|@HAVE_LIBGIT2[@]|$(HAVE_LIBGIT2)|g' \ -e 's|@HAVE_PTHREAD_BARRIER[@]|$(HAVE_PTHREAD_BARRIER)|g' \ $(srcdir)/gnuastro.h.in >> $@.tmp chmod a-w $@.tmp mv $@.tmp $@ gnuastro.pc: Makefile $(srcdir)/gnuastro.pc.in rm -f $@ $@.tmp $(SED) \ -e 's|@prefix[@]|$(prefix)|g' \ -e 's|@exec_prefix[@]|$(exec_prefix)|g' \ -e 's|@libdir[@]|$(libdir)|g' \ -e 's|@includedir[@]|$(includedir)|g' \ -e 's|@LIBS[@]|$(LIBS)|g' \ -e 's|@VERSION[@]|$(VERSION)|g' \ '$(srcdir)/$@.in' >> $@.tmp chmod a-w $@.tmp mv $@.tmp $@ gnuastro-0.2.33-8a3b/lib/gnuastro/0000755000175000017500000000000013004464724013611 500000000000000gnuastro-0.2.33-8a3b/lib/gnuastro/README0000644000175000017500000000127312774162326014422 00000000000000GNU Astronomy Utilities library header files ============================================ This directory contins Gnuastro's installed library header files. Once installed, these headers will be installed in the specified '$(prefix)/include/gnuastro' directory (the value of '$(prefix)' can be set at configure time, see the "Installation directory" of the Gnuastro book for more). Inside of Gnuastro, the directory is given the same name to make Gnuastro's internal code similar to what a user would use in their own programs once the header files are installed. The headers that are not installed are kept in the parent directory of this directory mixed with the actual library `.c' source files.gnuastro-0.2.33-8a3b/lib/gnuastro/txtarray.h0000644000175000017500000000504012772171231015556 00000000000000/********************************************************************* txtarray -- Convert a text file table to a C array. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_TXTARRAY_H__ #define __GAL_TXTARRAY_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Simple macros: */ #define GAL_TXTARRAY_LOG "txtarray.log" /* Read a text table file into a double C array. Some tables might have non-number elements, if so, they are put into replacements. Replacements is an array of strings (pointers to characters) similar to argv, since we need to allocate it inside this function you have to give its pointer, hence three dereferences. */ void gal_txtarray_txt_to_array(char *filename, double **array, size_t *s0, size_t *s1); void gal_txtarray_printf_format(int numcols, char **fmt, int *int_cols, int *accu_cols, int *space, int *prec, char forg); void gal_txtarray_array_to_txt(double *array, size_t s0, size_t s1, char *comments, int *int_cols, int *accu_cols, int *space, int *prec, char forg, const char *filename); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_TXTARRAY_H__ */ gnuastro-0.2.33-8a3b/lib/gnuastro/wcs.h0000644000175000017500000000422013001632540014462 00000000000000/********************************************************************* Functions to that only use WCSLIB's functions, not related to FITS. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_WCS_H__ #define __GAL_WCS_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ void gal_wcs_xy_array_to_radec(struct wcsprm *wcs, double *xy, double *radec, size_t number, size_t width); void gal_wcs_radec_array_to_xy(struct wcsprm *wcs, double *radec, double *xy, size_t number, size_t width); double gal_wcs_angular_distance_deg(double r1, double d1, double r2, double d2); void gal_wcs_pixel_scale_deg(struct wcsprm *wcs, double *dx, double *dy); double gal_wcs_pixel_area_arcsec2(struct wcsprm *wcs); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_WCS_H__ */ gnuastro-0.2.33-8a3b/lib/gnuastro/threads.h0000644000175000017500000000726213001632540015331 00000000000000/********************************************************************* Functions to facilitate using threads. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_THREADS_H__ #define __GAL_THREADS_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include /* When this header is included within Gnuastro's building process, `IN_GNUASTRO_BUILD' is defined. In the build process, installation information (in particular `GAL_GNUASTRO_HAVE_PTHREAD_BARRIER' that we need below) is kept in `config.h'. When building a user's programs, this information is kept in `gnuastro/gnuastro.h'. Note that all `.c' files must start with the inclusion of `config.h' and that `gnuastro/gnuastro.h' is only created at installation time (not present during the building of Gnuastro).*/ #ifndef IN_GNUASTRO_BUILD #include #endif /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Constant to use for non-existant index */ #define GAL_THREADS_NON_THRD_INDEX (size_t)(-1) /*****************************************************************/ /********* Implementation of pthread_barrier ***************/ /*****************************************************************/ #if GAL_GNUASTRO_HAVE_PTHREAD_BARRIER == 0 /* Integer number of nano-seconds that `pthread_barrier_destroy' should wait for a check to see if all barriers have been reached. */ #define GAL_THREADS_BARRIER_DESTROY_NANOSECS 1000 typedef int pthread_barrierattr_t; typedef struct { pthread_mutex_t mutex; pthread_cond_t cond; size_t count; size_t limit; size_t condfinished; } pthread_barrier_t; int pthread_barrier_init(pthread_barrier_t *b, pthread_barrierattr_t *attr, unsigned int limit); int pthread_barrier_wait(pthread_barrier_t *b); int pthread_barrier_destroy(pthread_barrier_t *b); #endif /* GAL_GNUASTRO_HAVE_PTHREAD_BARRIER == 0 */ /*****************************************************************/ /**************** gnuastro functions ******************/ /*****************************************************************/ void gal_threads_dist_in_threads(size_t numactions, size_t numthreads, size_t **outthrds, size_t *outthrdcols); void gal_threads_attr_barrier_init(pthread_attr_t *attr, pthread_barrier_t *b, size_t limit); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_THREADS_H__ */ gnuastro-0.2.33-8a3b/lib/gnuastro/statistics.h0000644000175000017500000002261612772171231016102 00000000000000/********************************************************************* Statistical functions. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_STATISTICS_H__ #define __GAL_STATISTICS_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Maximum number of tests for sigma-clipping convergence */ #define GAL_STATISTICS_MAX_SIG_CLIP_CONVERGE 50 /**************************************************************** ***************** Mininum and Maximum ******************** ****************************************************************/ void gal_statistics_long_non_blank_min(long *in, size_t size, long *min, long blank); void gal_statistics_long_non_blank_max(long *in, size_t size, long *max, long blank); void gal_statistics_float_min(float *in, size_t size, float *min); void gal_statistics_float_max(float *in, size_t size, float *max); void gal_statistics_double_min(double *in, size_t size, double *min); double gal_statistics_double_min_return(double *in, size_t size); void gal_statistics_double_max(double *in, size_t size, double *max); double gal_statistics_double_max_return(double *in, size_t size); void gal_statistics_float_max_masked(float *in, unsigned char *mask, size_t size, float *max); void gal_statistics_float_second_max(float *in, size_t size, float *secondmax); void gal_statistics_float_second_min(float *in, size_t size, float *secondmin); void gal_statistics_f_min_max(float *in, size_t size, float *min, float *max); void gal_statistics_d_min_max(double *in, size_t size, double *min, double *max); void gal_statistics_d_max_with_index(double *in, size_t size, double *max, size_t *index); void gal_statistics_f_max_with_index(float *in, size_t size, float *max, size_t *index); void gal_statistics_d_min_with_index(double *in, size_t size, double *min, size_t *index); void gal_statistics_f_min_with_index(float *in, size_t size, float *min, size_t *index); /**************************************************************** ***************** Sum ******************** ****************************************************************/ float gal_statistics_float_sum(float *in, size_t size); float gal_statistics_float_sum_num(float *in, size_t *size); float gal_statistics_float_sum_squared(float *in, size_t size); float gal_statistics_float_sum_mask(float *in, unsigned char *mask, size_t size, size_t *nsize); float gal_statistics_float_sum_mask_l(float *in, long *mask, size_t size, size_t *nsize); float gal_statistics_float_sum_squared_mask(float *in, unsigned char *mask, size_t size, size_t *nsize); float gal_statistics_float_sum_squared_mask_l(float *in, long *mask, size_t size, size_t *nsize); /**************************************************************** ***************** Average and ******************** **************** Standard deviation ******************** ****************************************************************/ float gal_statistics_float_average(float *in, size_t size); double gal_statistics_double_average(double *in, size_t size); void gal_statistics_f_ave(float *in, size_t size, float *ave, unsigned char *mask); void gal_statistics_f_ave_l(float *in, size_t size, float *ave, long *mask); void gal_statistics_f_ave_std(float *in, size_t size, float *ave, float *std, unsigned char *mask); void gal_statistics_f_ave_std_l(float *in, size_t size, float *ave, float *std, long *mask); /**************************************************************** ***************** Median ****************** ****************************************************************/ float gal_statistics_median(float *array, size_t insize); double gal_statistics_median_double_in_place(double *array, size_t insize); /**************************************************************** ******** Histogram and Cumulative Frequency Plot ******* ****************************************************************/ void gal_statistics_set_bins(float *sorted, size_t size, size_t numbins, float min, float max, float onebinvalue, float quant, float **obins); void gal_statistics_histogram(float *sorted, size_t size, float *bins, size_t numbins, int normhist, int maxhistone); void gal_statistics_cumulative_fp(float *sorted, size_t size, float *bins, size_t numbins, int normcfp); void gal_statistics_save_hist(float *sorted, size_t size, size_t numbins, char *filename, char *comment); /**************************************************************** ***************** Quantiles ******************** ****************************************************************/ size_t gal_statistics_index_from_quantile(size_t size, float quant); /**************************************************************** ***************** Sigma clip ******************** ****************************************************************/ int gal_statistics_sigma_clip_converge(float *array, int o1_n0, size_t num_elem, float sigma_multiple, float accuracy, float *outave, float *outmed, float *outstd, int print); int gal_statistics_sigma_clip_certain_num(float *array, int o1_n0, size_t num_elem, float sigma_multiple, size_t numtimes, float *outave, float *outmed, float *outstd, int print); /****************************************************************/ /************* Identify outliers ****************/ /****************************************************************/ void gal_statistics_remove_outliers_flat_cdf(float *sorted, size_t *outsize); /****************************************************************/ /************* Mode ****************/ /****************************************************************/ #define GAL_STATISTICS_MODE_LOW_QUANTILE 0.01f #define GAL_STATISTICS_MODE_HIGH_QUANTILE 0.51f #define GAL_STATISTICS_MODE_SYM_GOOD 0.2f #define GAL_STATISTICS_MODE_LOW_QUANT_GOOD 0.02f #define GAL_STATISTICS_MODE_SYMMETRICITY_LOW_QUANT 0.01f struct gal_statistics_mode_params { float *sorted; /* Sorted array to be used. */ size_t size; /* Number of elements in the sorted array. */ size_t lowi; /* Lower quantile of interval. */ size_t midi; /* Middle quantile of interval. */ size_t midd; /* Middle index of inteval. */ size_t highi; /* Higher quantile of interval. */ float tolerance; /* Tolerance level to terminate search. */ size_t numcheck; /* Number of pixels after mode to check. */ size_t interval; /* Interval to check pixels. */ float errorstdm; /* Multiple of standard deviation. */ }; void gal_statistics_mode_mirror_plots(float *sorted, size_t size, size_t mirrorindex, float min, float max, size_t numbins, char *histsname, char *cfpsname, float mirrorplotdist); float gal_statistics_mode_value_from_sym(float *sorted, size_t size, size_t modeindex, float sym); void gal_statistics_mode_index_in_sorted(float *sorted, size_t size, float errorstdm, size_t *modeindex, float *modesym); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_STATISTICS_H__ */ gnuastro-0.2.33-8a3b/lib/gnuastro/spatialconvolve.h0000644000175000017500000000704712772171231017122 00000000000000/********************************************************************* SpatialConvolve - Convolve an image in the spatial domain. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_SPATIALCONVOLVE_H__ #define __GAL_SPATIALCONVOLVE_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include /* For pthread_barrier_t: */ /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Main structure: */ struct gal_spatialconvolve_params { /* General input parameters: */ float *input; /* Input image array. */ float *kernel; /* Kernel array. */ float *out; /* Output image. */ size_t is0; /* Image size along first C axis. */ size_t is1; /* Image size along second C axis. */ size_t ks0; /* Kernel size along first C axis. */ size_t ks1; /* Kernel size along second C axis. */ int edgecorrection; /* Correct the edges of the image. */ long fpixel_i[2]; /* First pixel in input image. */ long lpixel_i[2]; /* Last pixel in input image. */ long fpixel_o[2]; /* First pixel in kernel. */ long lpixel_o[2]; /* Last pixel in kernel. */ /* Thread parameters. */ size_t numthreads; /* Number of threads. */ size_t *indexs; /* Indexs to be used in this thread. */ pthread_barrier_t *b; /* Barrier to keep threads waiting. */ }; /* Functions: */ void gal_spatialconvolve_pparams(float *input, size_t is0, size_t is1, float *kernel, size_t ks0, size_t ks1, size_t nt, int edgecorrection, float *out, size_t *indexs, struct gal_spatialconvolve_params *scp); void * gal_spatialconvolve_thread(void *inparam); void gal_spatialconvolve_convolve(float *input, size_t is0, size_t is1, float *kernel, size_t ks0, size_t ks1, size_t nt, int edgecorrection, float **out); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_SPATIALCONVOLVE_H__ */ gnuastro-0.2.33-8a3b/lib/gnuastro/qsort.h0000644000175000017500000000433512772171231015056 00000000000000/********************************************************************* forqsort -- Functions used by qsort to sort an array. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_QSORT_H__ #define __GAL_QSORT_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Pointer used to sort the indexs of an array based on their flux (value in this array). */ extern float *gal_qsort_index_arr; int gal_qsort_index_float_decreasing(const void * a, const void * b); int gal_qsort_int_decreasing(const void * a, const void * b); int gal_qsort_int_increasing(const void * a, const void * b); int gal_qsort_float_decreasing(const void * a, const void * b); int gal_qsort_float_increasing(const void * a, const void * b); int gal_qsort_double_decreasing(const void * a, const void * b); int gal_qsort_double_increasing(const void * a, const void * b); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_QSORT_H__ */ gnuastro-0.2.33-8a3b/lib/gnuastro/polygon.h0000644000175000017500000000435612772171231015400 00000000000000/********************************************************************* Polygon related functions and macros. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_POLYGON_H__ #define __GAL_POLYGON_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ #define GAL_POLYGON_MAX_CORNERS 50 #define GAL_POLYGON_ROUND_ERR 1e-5 /***************************************************************/ /************** Function declarations ******************/ /***************************************************************/ void gal_polygon_ordered_corners(double *in, size_t n, size_t *ordinds); double gal_polygon_area(double *v, size_t n); int gal_polygon_pin(double *v, double *p, size_t n); int gal_polygon_ppropin(double *v, double *p, size_t n); void gal_polygon_clip(double *s, size_t n, double *c, size_t m, double *o, size_t *numcrn); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_POLYGON_H__ */ gnuastro-0.2.33-8a3b/lib/gnuastro/mesh.h0000644000175000017500000001744112772171231014644 00000000000000/********************************************************************* meshgrid -- Create a mesh grid ready for multithreaded analysis. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_MESH_H__ #define __GAL_MESH_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Operations to do on each mesh. If input parameters are needed (for example the quantile), they are given as other argument(s) to the fillcharray function. */ #define GAL_MESH_MAX_NUM_CHARRAY 2 /* Maximum number of charrays. */ #define GAL_MESH_INTERP_ALL 1 /* Interpolate over the whole image as one. */ #define GAL_MESH_INTERP_CHANNEL 2 /* Interpolate over each channel individually.*/ /* The minimum number of acceptable nearest pixels. */ #define GAL_MESH_MIN_ACCEPTABLE_NEAREST 3 struct gal_mesh_thread_params { /* For convolve: */ float *conv; /* The convolved array. */ size_t *chbrd; /* Bordering x and y values all channels. */ /* For all: */ struct gal_mesh_params *mp; /* Pointer to gal_mesh_params structure. */ size_t id; /* The thread ID starting from zero. */ }; struct gal_mesh_params { /* Image: */ void *img; /* Input image array. */ size_t s0; /* Height of input image. */ size_t s1; /* Width of input image. */ /* Threads: */ size_t numthreads; /* Number of CPU threads. */ size_t *indexs; /* 2D array of mesh indexs for each thread. */ size_t thrdcols; /* The number of columns in indexs array. */ pthread_barrier_t b; /* pthreads barrier for running threads. */ /* Channel(s): */ size_t nch; /* Total number of channels. */ size_t nch1; /* Number of channels along first FITS axis. */ size_t nch2; /* Number of channels along first FITS axis. */ size_t gs0; /* Number of meshes on axis 0 in each channel. */ size_t gs1; /* Number of meshes on axis 1 in each channel. */ /* Meshs: */ float lastmeshfrac; /* Last mesh fraction of size, to add new. */ size_t meshsize; /* Size of each mesh. */ size_t nmeshc; /* Number of meshes in each channel. */ size_t nmeshi; /* Number of meshes in all image. */ size_t *start; /* Starting pixel for each mesh. */ size_t *types; /* The type of each mesh. */ size_t *chindex; /* The index of each mesh in its channel. */ size_t *imgindex; /* The index of each mesh in the image. */ size_t maxs0; /* Maximum number of rows in all types. */ size_t maxs1; /* Maximum number of columns in all types. */ /* garrays: */ int ngarrays; /* Number of garrays in this run. */ float *garray1; /* Either equal to cgarray1 or fgarray1. */ float *garray2; /* Either equal to cgarray2 or fgarray2. */ float *cgarray1; /* In cgarray1 or cgarray2, the meshs in each */ float *cgarray2; /* channel are contiguous. */ float *fgarray1; /* In fgarray1 or fgarray2, we have contiguous */ float *fgarray2; /* meshs in the full image. Ignore channels.*/ /* Operate on each mesh: */ void *params; /* Pointer to parameters structure of caller. */ void *oneforall; /* One array that can contain all the meshs. */ /* Interpolation: */ float mirrordist; /* For finding the mode. Distance after mirror.*/ float minmodeq; /* Minimum acceptable quantile for the mode. */ unsigned char *byt; /* To keep track of pixels already checked. */ size_t numnearest; /* Number of the nearest pixels for interp. */ float *nearest1; /* Array keeping nearest pixels for garray1. */ float *nearest2; /* Array keeping nearest pixels for garray2. */ int interponlyblank; /* Only interpolate over blank pixels. */ float *outgarray1; /* The interpolated garray1. */ float *outgarray2; /* The interpolated garray2. */ int fullinterpolation; /* ==1: Ignore channels in interpolation. */ char *errstart; /* First sentence for error message. */ /* Smoothing: */ size_t smoothwidth; /* Width of smoothing kernel. */ int fullsmooth; /* ==1: Ignore channels in smoothing. */ /* Convolution: */ float *kernel; /* Convolution kernel. */ size_t ks0; /* Size of kernel along first C axis. */ size_t ks1; /* Size of kernel along second C axis. */ int fullconvolution; /* ==1: Convove over all channels. */ /* Mesh types and information: */ int meshbasedcheck; /* ==1: use one pixel for each mesh in checks. */ size_t ts0[4]; /* Size (along first FITS axis) of mesh types. */ size_t ts1[4]; /* Size (along second FITS axis) of mesh types.*/ }; size_t gal_mesh_ch_based_id_from_gid(struct gal_mesh_params *mp, size_t gid); size_t gal_mesh_gid_from_ch_based_id(struct gal_mesh_params *mp, size_t chbasedid); size_t gal_mesh_img_xy_to_mesh_id(struct gal_mesh_params *mp, size_t x, size_t y); void gal_mesh_check_mesh_id(struct gal_mesh_params *mp, long **out); void gal_mesh_check_garray(struct gal_mesh_params *mp, float **out1, float **out2); void gal_mesh_value_file(struct gal_mesh_params *mp, char *filename, char *extname1, char *extname2, struct wcsprm *wcs, char *spack_string); void gal_mesh_full_garray(struct gal_mesh_params *mp, int reverse); void gal_mesh_make_mesh(struct gal_mesh_params *mp); void gal_mesh_free_mesh(struct gal_mesh_params *mp); void gal_mesh_operate_on_mesh(struct gal_mesh_params *mp, void *(*meshfunc)(void *), size_t oneforallsize, int makegarray2, int initialize); void gal_mesh_interpolate(struct gal_mesh_params *mp, char *errstart); void gal_mesh_smooth(struct gal_mesh_params *mp); void gal_mesh_spatial_convolve_on_mesh(struct gal_mesh_params *mp, float **conv); void gal_mesh_change_to_full_convolution(struct gal_mesh_params *mp, float *conv); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_MESH_H__ */ gnuastro-0.2.33-8a3b/lib/gnuastro/linkedlist.h0000644000175000017500000001366712772171231016060 00000000000000/********************************************************************* Functions for linked lists. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_SLL_H__ #define __GAL_SLL_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /******************* float: */ struct gal_linkedlist_fll { float v; struct gal_linkedlist_fll *next; }; void gal_linkedlist_print_fll_array(struct gal_linkedlist_fll **afll, size_t num); void gal_linkedlist_add_to_fll(struct gal_linkedlist_fll **list, float value); void gal_linkedlist_pop_from_fll(struct gal_linkedlist_fll **list, float *value); size_t gal_linkedlist_num_in_fll(struct gal_linkedlist_fll *list); void gal_linkedlist_fll_to_array(struct gal_linkedlist_fll *list, float **f, size_t *num); void gal_linkedlist_free_fll(struct gal_linkedlist_fll *list); void gal_linkedlist_free_fll_array(struct gal_linkedlist_fll **afll, size_t num); /******************* Two doubles (for coordinates) */ struct gal_linkedlist_tdll { double a; double b; struct gal_linkedlist_tdll *next; }; void gal_linkedlist_add_to_tdll(struct gal_linkedlist_tdll **list, double a, double b); void gal_linkedlist_pop_from_tdll(struct gal_linkedlist_tdll **list, double *a, double *b); size_t gal_linkedlist_num_int_dll(struct gal_linkedlist_tdll *list); void gal_linkedlist_tdll_to_array_inv(struct gal_linkedlist_tdll *list, double **d, size_t *num); void gal_linkedlist_free_tdll(struct gal_linkedlist_tdll *list); /******************* String: */ struct gal_linkedlist_stll { char *v; struct gal_linkedlist_stll *next; }; void gal_linkedlist_add_to_stll(struct gal_linkedlist_stll **list, char *value); void gal_linkedlist_pop_from_stll(struct gal_linkedlist_stll **list, char **value); void gal_linkedlist_reverse_stll(struct gal_linkedlist_stll **list); void gal_linkedlist_print_stll(struct gal_linkedlist_stll *list); size_t gal_linkedlist_num_in_stll(struct gal_linkedlist_stll *list); /******************* size_t: */ struct gal_linkedlist_sll { size_t v; struct gal_linkedlist_sll *next; }; void gal_linkedlist_add_to_sll(struct gal_linkedlist_sll **list, size_t value); void gal_linkedlist_pop_from_sll(struct gal_linkedlist_sll **list, size_t *value); size_t gal_linkedlist_num_in_sll(struct gal_linkedlist_sll *list); void gal_linkedlist_print_sll(struct gal_linkedlist_sll *list); void gal_linkedlist_sll_to_array(struct gal_linkedlist_sll *list, size_t **s, size_t *num, int inverse); void gal_linkedlist_free_sll(struct gal_linkedlist_sll *list); /******************* Ordered size_t: */ struct gal_linkedlist_osll { size_t v; /* The actual value. */ float s; /* The parameter to sort by. */ struct gal_linkedlist_osll *next; }; void gal_linkedlist_add_to_osll(struct gal_linkedlist_osll **list, size_t value, float tosort); void gal_linkedlist_pop_from_osll(struct gal_linkedlist_osll **list, size_t *value, float *sortvalue); void gal_linkedlist_osll_into_sll(struct gal_linkedlist_osll *in, struct gal_linkedlist_sll **out); /******************* Two way ordered size_t: */ struct gal_linkedlist_tosll { size_t v; float s; struct gal_linkedlist_tosll *prev; struct gal_linkedlist_tosll *next; }; void gal_linkedlist_print_tosll(struct gal_linkedlist_tosll *largest, struct gal_linkedlist_tosll *smallest); void gal_linkedlist_add_to_tosll_end(struct gal_linkedlist_tosll **largest, struct gal_linkedlist_tosll **smallest, size_t value, float tosort); void gal_linkedlist_pop_from_tosll_start(struct gal_linkedlist_tosll **lartest, struct gal_linkedlist_tosll **smallest, size_t *value, float *tosort); void gal_linkedlist_smallest_tosll(struct gal_linkedlist_tosll *largest, struct gal_linkedlist_tosll **smallest); void gal_linkedlist_tosll_into_sll(struct gal_linkedlist_tosll *in, struct gal_linkedlist_sll **out); void gal_linkedlist_tosll_free(struct gal_linkedlist_tosll *largest); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_LINKEDLIST_H__ */ gnuastro-0.2.33-8a3b/lib/gnuastro/git.h0000644000175000017500000000322513001632540014455 00000000000000/********************************************************************* Functions to facilitate using the Git library. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_GIT_H__ #define __GAL_GIT_H__ #if GAL_GNUASTRO_HAVE_LIBGIT2 == 1 #include #endif /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Only make the Git definitions if the system has LIBGIT2, */ char * gal_git_describe(); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_GIT_H__ */ gnuastro-0.2.33-8a3b/lib/gnuastro/fits.h0000644000175000017500000002144613002475046014653 00000000000000/********************************************************************* Functions to convert a FITS array to a C array and vice versa. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_FITS_H__ #define __GAL_FITS_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include #include #include #include #include #include #include #include #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Order is based on the CFITSIO manual. Note that for the unsigned types or small types (like char), the maximum value is considered as a blank value, since the minimum value of an unsigned type is zero and zero is often meaningful in contexts were unsigned values are used. */ #define GAL_FITS_STRING_BLANK NULL #define GAL_FITS_BYTE_BLANK UCHAR_MAX #define GAL_FITS_LOGICAL_BLANK SCHAR_MAX #define GAL_FITS_SHORT_BLANK INT16_MIN #define GAL_FITS_LONG_BLANK INT32_MIN #define GAL_FITS_LLONG_BLANK INT64_MIN #define GAL_FITS_FLOAT_BLANK NAN #define GAL_FITS_DOUBLE_BLANK NAN #define GAL_FITS_INT_BLANK INT_MIN #define GAL_FITS_SBYTE_BLANK SCHAR_MAX #define GAL_FITS_UINT_BLANK UINT_MAX #define GAL_FITS_USHORT_BLANK USHRT_MAX #define GAL_FITS_ULONG_BLANK ULONG_MAX /************************************************************* ****************** Basic ******************* *************************************************************/ void gal_fits_io_error(int status, char *message); int gal_fits_name_is_fits(char *name); int gal_fits_suffix_is_fits(char *suffix); /************************************************************* ****************** Header ****************** *************************************************************/ /* To create a linked list of headers. */ struct gal_fits_key_ll { int kfree; /* ==1, free keyword name. */ int vfree; /* ==1, free keyword value. */ int cfree; /* ==1, free comment. */ int datatype; /* Keyword value datatype. */ char *keyname; /* Keyword Name. */ void *value; /* Keyword value. */ char *comment; /* Keyword comment. */ char *unit; /* Keyword unit. */ struct gal_fits_key_ll *next; /* Pointer next keyword. */ }; struct gal_fits_key { int status; /* CFITSIO status. */ char *keyname; /* Name of keyword. */ int datatype; /* Type of keyword value. */ char str[FLEN_VALUE]; /* String value. */ unsigned char u; /* Byte value. */ short s; /* Short integer value. */ long l; /* Long integer value. */ LONGLONG L; /* Long Long value. */ float f; /* Float value. */ double d; /* Double value. */ }; void gal_fits_read_keywords(char *filename, char *hdu, struct gal_fits_key *out, size_t num); void gal_fits_add_to_key_ll(struct gal_fits_key_ll **list, int datatype, char *keyname, int kfree, void *value, int vfree, char *comment, int cfree, char *unit); void gal_fits_add_to_key_ll_end(struct gal_fits_key_ll **list, int datatype, char *keyname, int kfree, void *value, int vfree, char *comment, int cfree, char *unit); void gal_fits_file_name_in_keywords(char *keynamebase, char *filename, struct gal_fits_key_ll **list); void gal_fits_add_wcs_to_header(fitsfile *fptr, char *wcsheader, int nkeyrec); void gal_fits_update_keys(fitsfile *fptr, struct gal_fits_key_ll **keylist); void gal_fits_write_keys_version(fitsfile *fptr, struct gal_fits_key_ll *headers, char *spack_string); /************************************************************* ****************** Read/Write ***************** *************************************************************/ void * gal_fits_datatype_blank(int datatype); void gal_fits_convert_blank(void *array, int bitpix, size_t size, void *value); void gal_fits_blank_to_value(void *array, int datatype, size_t size, void *value); int gal_fits_bitpix_to_datatype(int bitpix); void gal_fits_img_bitpix_size(fitsfile *fptr, int *bitpix, long *naxis); void gal_fits_read_hdu(char *filename, char *hdu, unsigned char img0_tab1, fitsfile **outfptr); void * gal_fits_datatype_alloc(size_t size, int datatype); size_t gal_fits_datatype_size(int datatype); void gal_fits_change_type(void *in, int inbitpix, size_t size, int anyblank, void **out, int outbitpix); void gal_fits_num_hdus(char *filename, int *numhdu); void gal_fits_read_wcs_from_pointer(fitsfile *fptr, int *nwcs, struct wcsprm **wcs, size_t hstart, size_t hend); void gal_fits_read_wcs(char *filename, char *hdu, size_t hstartwcs, size_t hendwcs, int *nwcs, struct wcsprm **wcs); int gal_fits_hdu_to_array(char *filename, char *hdu, int *bitpix, void **array, size_t *s0, size_t *s1); void gal_fits_array_to_file(char *filename, char *hdu, int bitpix, void *array, size_t s0, size_t s1, int anyblank, struct wcsprm *wcs, struct gal_fits_key_ll *headers, char *spack_string); void gal_fits_atof_correct_wcs(char *filename, char *hdu, int bitpix, void *array, size_t s0, size_t s1, char *wcsheader, int wcsnkeyrec, double *crpix, char *spack_string); /**************************************************************/ /********** Table ************/ /**************************************************************/ int gal_fits_tform_to_datatype(char tform); void gal_fits_table_size(fitsfile *fitsptr, size_t *nrows, size_t *ncols); int gal_fits_table_type(fitsfile *fptr); /**************************************************************/ /********** Check prepare file ************/ /**************************************************************/ void gal_fits_file_or_ext_name(char *inputname, char *inhdu, int othernameset, char **othername, char *ohdu, int ohduset, char *type); void gal_fits_set_mask_name(char *inputname, char **maskname, char *inhdu, char *mhdu); void gal_fits_file_to_double(char *inputname, char *maskname, char *inhdu, char *mhdu, double **img, int *inbitpix, int *anyblank, size_t *ins0, size_t *ins1); void gal_fits_file_to_float(char *inputname, char *maskname, char *inhdu, char *mhdu, float **img, int *inbitpix, int *anyblank, size_t *ins0, size_t *ins1); void gal_fits_file_to_long(char *inputname, char *inhdu, long **img, int *inbitpix, int *anyblank, size_t *ins0, size_t *ins1); void gal_fits_prep_float_kernel(char *inputname, char *inhdu, float **kernel, size_t *ins0, size_t *ins1); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_FITS_H__ */ gnuastro-0.2.33-8a3b/lib/gnuastro/box.h0000644000175000017500000000406412772171231014475 00000000000000/********************************************************************* overlap -- Find the overlap of a region and an image. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_BOX_H__ #define __GAL_BOX_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* IMPORTANT NOTE: All the axises are based on the FITS standard, NOT C. */ void gal_box_ellipse_in_box(double a, double b, double theta_rad, long *width); void gal_box_border_from_center(double xc, double yc, long *width, long *fpixel, long *lpixel); int gal_box_overlap(long *naxes, long *fpixel_i, long *lpixel_i, long *fpixel_o, long *lpixel_o); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_BOX_H__ */ gnuastro-0.2.33-8a3b/lib/gnuastro/array.h0000644000175000017500000000757012772171231015030 00000000000000/********************************************************************* Functions to manipulate arrays. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_ARRAY_H__ #define __GAL_ARRAY_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ void gal_array_uchar_init_on_region(unsigned char *in, const unsigned char v, size_t start, size_t s0, size_t s1, size_t is1); void gal_array_long_init(long *in, size_t size, const long v); void gal_array_long_init_on_region(long *in, const long v, size_t start, size_t s0, size_t s1, size_t is1); void gal_array_uchar_copy(unsigned char *in, size_t size, unsigned char **out); void gal_array_float_copy(float *in, size_t size, float **out); void gal_array_float_copy_noalloc(float *in, size_t size, float *out); void gal_array_fset_const(float *in, size_t size, float a); void gal_array_freplace_value(float *in, size_t size, float from, float to); void gal_array_freplace_nonnans(float *in, size_t size, float to); void gal_array_no_nans(float *in, size_t *size); void gal_array_no_nans_double(double *in, size_t *size); void gal_array_uchar_replace(unsigned char *in, size_t size, unsigned char from, unsigned char to); void gal_array_fmultip_const(float *in, size_t size, float a); void gal_array_fsum_const(float *in, size_t size, float a); float * gal_array_fsum_arrays(float *in1, float *in2, size_t size); void gal_array_dmultip_const(double *in, size_t size, double a); void gal_array_dmultip_arrays(double *in1, double *in2, size_t size); void gal_array_ddivide_const(double *in, size_t size, double a); void gal_array_dconst_divide(double *in, size_t size, double a); void gal_array_ddivide_arrays(double *in1, double *in2, size_t size); void gal_array_dsum_const(double *in, size_t size, double a); void gal_array_dsum_arrays(double *in1, double *in2, size_t size); void gal_array_dsubtract_const(double *in, size_t size, double a); void gal_array_dconst_subtract(double *in, size_t size, double a); void gal_array_dsubtract_arrays(double *in1, double *in2, size_t size); void gal_array_dpower_const(double *in, size_t size, double a); void gal_array_dconst_power(double *in, size_t size, double a); void gal_array_dpower_arrays(double *in1, double *in2, size_t size); void gal_array_dlog_array(double *in1, size_t size); void gal_array_dlog10_array(double *in1, size_t size); void gal_array_dabs_array(double *in1, size_t size); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_ARRAY_H__ */ gnuastro-0.2.33-8a3b/lib/gnuastro/gnuastro.h0000444000175000017500000000351613004464665015553 00000000000000/********************************************************************* Functions dealing with general aspects of all Gnuastro. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_GNUASTRO_H__ #define __GAL_GNUASTRO_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* Macros. In gnuastro.h.in, the values in `@' --- `@'', will be replaced with installation specific values. */ #define GAL_GNUASTRO_VERSION "0.2.33-8a3b" #define GAL_GNUASTRO_HAVE_LIBGIT2 1 #define GAL_GNUASTRO_HAVE_PTHREAD_BARRIER 1 /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_GNUASTRO_H__ */ gnuastro-0.2.33-8a3b/.autom4te.cfg0000644000175000017500000000176012722534072013426 00000000000000# Configuration file for autom4te # =============================== # autom4te is used to create the familiar `./configure' script from # configure.ac (hand written by Gnuastro developers). autom4te is # called during the bootstrapping process (see README-hacking, or the # "Bootstrapping" section in the manual). # # To speed up the process, a directory (`autom4te.cache') is created # which keeps cache information which can speed up its next call. But # this directory is built in the top Gnuastro directory which just # redundantly fills it up with a non-edited directory. So through this # configuration file, we are asking autom4te to make its cache # directory within the bootstrapped directory to keep things on the # top directory clean. # We are using the Autoconf manual's "Customizing autom4te" and # "Invoking autom4te" sections as a reference for this file. begin-language: "Autoconf-without-aclocal-m4" args: --cache=./bootstrapped/autom4te.cache end-language: "Autoconf-without-aclocal-m4"gnuastro-0.2.33-8a3b/tmpfs-config-make0000755000175000017500000000646113002500764014356 00000000000000#! /bin/sh # This script will configure and build Gnuastro in parallel within a # temporary tmpfs directory in the RAM. Please see the "Configure and build # in RAM" section of the Gnuastro book/documentation for a full # explanation. # # Original author: Mohammad Akhlaghi # Contributing author(s): # Mosè Giordano # Copyright (C) 2016, Free Software Foundation, Inc. # # Gnuastro is free software: you can redistribute it and/or modify it under # the terms of the GNU General Public License as published by the Free # Software Foundation, either version 3 of the License, or (at your option) # any later version. # # Gnuastro is distributed in the hope that it will be useful, but WITHOUT # ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or # FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for # more details. # # You should have received a copy of the GNU General Public License along # with Gnuastro. If not, see . # Set the variables: NUM_THREADS=8 TMPDIR=/dev/shm # Check if TMPDIR exists if [ ! -d $TMPDIR ]; then echo "$TMPDIR doesn't exist. Aborted." exit 1 fi # Keep the address of this source directory (where this script is being run # from) which we will need later. srcdir=$(pwd) # Set the build directory name in tmpfs. If the .version file exists, use # it to allow multiple version builds there (which might happen during # development). basedir=$(basename -- "$srcdir") if [ -f .version ]; then build_dir=$TMPDIR/"$basedir"-$(cat .version) else build_dir=$TMPDIR/"$basedir" fi # Make the build directory in tmpfs (if it doesn't already exist). if [ ! -d $build_dir ]; then mkdir $build_dir fi # Make a symbolic link to the tmpfs build directory for users to easily # access the built files and also follow the progress. We are first # deleting any existing symbolic link and remaking it since the possible # deletion of $build_dir during the development can complicate the # pre-existing symbolic link. build_sym=build if [ -h $build_sym ]; then # Delete a harmless symbolic link, if present. rm $build_sym fi # Create the link only if the symbolic link doesn't exist. if [ ! -e $build_sym ]; then ln -s $build_dir $build_sym else echo "$build_sym already exists here and is not a symbolic link." echo "Aborted." exit 1 fi # Go into the build directory to start the configure and/or build: cd $build_dir # If a 'Makefile' doesn't exist, then configure Gnuastro. # # FOR DEBUGGING: uncomment the second half of this line. Gnuastro uses GNU # Libtool to build shared libraries for highly portable and maintainable # usage on a wide variety of systems. While this is great for binaries, it # can be a pain when trying to debug. For this reason, compilation of # shared libraries can be turned off by specifying the --disable-shared # option to configure. With static libraries, compilation (the `make' # command) will also significantly speed up. Also, by default (in # `configure.ac'), we have set optimization flags which have to be # cancelled in debugging. if [ ! -f Makefile ]; then $srcdir/configure --srcdir=$srcdir #--disable-shared CFLAGS="-g -O0" fi # Build Gnuastro in that directory with the specified number of threads make -kj$NUM_THREADS gnuastro-0.2.33-8a3b/.version0000644000175000017500000000001413004464663012604 000000000000000.2.33-8a3b gnuastro-0.2.33-8a3b/.dir-locals.el0000644000175000017500000000147512744764314013571 00000000000000;; This files contains Emacs Directory Local Variables. ;; ;; Emacs is an extensible, customizable, free/libre text editor. It ;; allows specification of certain settings that will be applied to ;; all files in current directory and its subdirectories. This is ;; useful in order to automatically enforce certain coding conventions ;; for all contributors of Gnuastro, like the maximum length of lines ;; or the number of spaces to be used for indentation. ;; ;; For more information see (info "(emacs) Directory Variables") ((nil (indent-tabs-mode . nil) ;; No tabs as indentation (fill-column . 75)) ;; 75-character wide lines (c-mode (c-basic-offset . 2) ;; 2 spaces of indentation (c-file-style . "gnu")) ;; GNU style for braces (makefile-mode (indent-tabs-mode . t)) ;; Real TABs are important in makefiles ) gnuastro-0.2.33-8a3b/genauthors0000755000175000017500000000625312771530354013237 00000000000000#! /bin/sh # # Generate a list of authors from the git repository, it will only # actually do anything if a .git file exists. Run like this: # # ./genauthors top/bin/dir # # Note that some authors might have changed their email addresses over # the course of their contributions to Gnuastro. Fortunately Git has a # great tool for that: the .mailmap file. It has already been included # in the source code and if any author changes their email address or # would want their name to be printed differently here, please use # that file. See the git-shortlog manpage for a complete explanation # of all the possible ways to do this. # # Original author: # Mohammad Akhlaghi # Contributing author(s): # Copyright (C) 2015, Free Software Foundation, Inc. # # Gnuastro is free software: you can redistribute it and/or modify it # under the terms of the GNU General Public License as published by the # Free Software Foundation, either version 3 of the License, or (at your # option) any later version. # # Gnuastro is distributed in the hope that it will be useful, but # WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU # General Public License for more details. # # You should have received a copy of the GNU General Public License # along with Gnuastro. If not, see . # Initial settings: set -o nounset # Stop if a variable is not set. set -o errexit # Stop if a program returns false. # Only do the job if a .git directory exists (recall that this script # is also present in the tar-ball with no .git directory and might be # run from there) if [ ! -d "$1/.git" ]; then echo "There is no Git repository in the source directory." echo "AUTHORS cannot be generated." exit 0 fi # Print a status report, since this will be run along with the large # number of bootstrap operations, it is best to tell the users since # it might take a few seconds. echo "Generating AUTHORS from the version controlled source..." # Make sure the .mailmap file is present in this directory, so Git can fix # the different email addresses and names of one person. Note that while # this is in the top source directory, it is possible for the source and # build directories to be different, and we have to be prepared for that. if [ ! -f .mailmap ]; then ln -s $1/.mailmap .mailmap fi # Set the version number. Note that this script is also run at the start of # the bootstrapping process. At that point we don't have the `.version' # file, so we will just rely on `.git describe'. Later during `make', this # scripot will be run again to set it using `git-version-gen'. if [ -f "$1/.version" ]; then gnuastroversion="Gnuastro "$(cat "$1/.version") else gnuastroversion=$(git --git-dir=$1/.git describe) fi # Print the top of the AUTHORS file. echo "GNU Astronomy Utilities (Gnuastro) authors ========================================== Generated for $gnuastroversion. Ordered by number of commits in the Git project history. " > $1/AUTHORS # Generate the aggregate list git --git-dir=$1/.git shortlog --summary --email --no-merges >> $1/AUTHORS gnuastro-0.2.33-8a3b/bootstrap.conf0000644000175000017500000001516612776533030014020 00000000000000# Bootstrap configuration for GNU Astronomy Utilities # # This file will be read by the ./bootstrap script and everything that # is defined here will be replaced with the variables defined # there. ./bootstrap is a script made by Gnulib in order to run Gnulib # and any other operation that is necessary to do on the version # controlled source prior to running ./configure. # # IMPORTANT NOTE(s) FOR GNUASTRO: # # - We have separated the variables defined here into three # categories as clearly seen below. The main reason is that if # Gnulib's template bootstrap.conf ever changes in the future, we # know exactly which parts we have modified for Gnuastro and so, # we can easily update this template. # # Original author: # Mosè Giordano # Contributing author(s): # Mohammad Akhlaghi # Copyright (C) 2016 Free Software Foundation, Inc. # # This program is free software: you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see . # Gnuastro specific configuration variables # ========================================= # # These are configurations that were added specifically for # bootstrapping Gnuastro, these variables were originally not in this # configuration file, we have copied them from the bootstrap script # since everything here is going to be replaced with the same variable # that was defined there. # Run the genauthors script to create the AUTHORS file which is # necessary in autoreconf. Recall that we have to satisfy the GNU # Coding Standards which require this file's existence and autoreconf # will complain if its not here. ./genauthors ./ # Extra options we want to have added to the execution of gnulib-tool # for Gnuastro. See the `gnulib_tool_options' variable in bootstrap # for the default options that will be used and as a template. gnulib_tool_option_extras="\ --with-tests\ --no-vc-files\ " # Redefine the base directories for output files. We don't want # imported files to be mixed up with hand-written Gnuastro # files. m4_base="bootstrapped/m4" doc_base="bootstrapped/doc" source_base="bootstrapped/lib" tests_base="bootstrapped/tests" build_aux="bootstrapped/build-aux" # This name will be appended to the Gnulib's Automake variables. By # default the ./bootstrap script takes the long package name as a # reference, but for Gnuastro, since the long package name contains a # space, it is replaced with astronomy-utilities, and so Automake will # complain (for example: bad characters in variable name # 'libastronomy-utilities_la_SOURCES'). So we are also redefining it # here. This name is irrelevant for the final process. gnulib_name="libgnu" # Processes to run after gnulib-tool and before autoreconf. bootstrap_post_import_hook() { # List of m4 files we need from the GNU Autoconf Archives (excluding the # `ax_' prefix and `.m4' suffix): neededm4s="pthread compare_version" # Get the necesssary Autoconf-archive macros. It is assumed that # autoconf-archives is cloned the same directory as gnulib. Therefore we # simply copy the desired m4 macros if an Autoconf-archive exists or # download it otherwise. if [ -f "$GNULIB_SRCDIR/../autoconf-archive/m4/ax_pthread.m4" ]; then for m4name in $neededm4s; do cp "$GNULIB_SRCDIR/../autoconf-archive/m4/ax_$m4name.m4" $m4_base/ done else # Choose the program to use to download files from the web. `curl' is # present in most GNU/Linux systems and OS X as well, `wget' is usually # present only on GNU/Linux systems. Since `curl' is available in more # systems, we first try if it's installed, otherwise we fallback on # `wget'. if type curl > /dev/null; then downloader="curl -o" else downloader="wget -O" fi for m4name in $neededm4s; do $downloader "$m4_base/ax_$m4name.m4" \ "http://git.savannah.gnu.org/gitweb/?p=autoconf-archive.git;a=blob_plain;f=m4/ax_$m4name.m4" || die "Failed to download ax_$m4name.m4!" done fi } # Run other necessary operations after all the default bootstrap # operations are complete. bootstrap_epilogue() { # Prepare all the figure formats for the various manual formats. cd doc/plotsrc make cd ../../ } # Configuration variable values for Gnuastro # ========================================== # # These are variables that were included in the gnulib's # bootstrap.conf template but have been given values specifically for # Gnuastro. # gnulib modules used by this package. gnulib_modules=" fdl math argp regex error nproc strcase gendocs git-version-gen " # Exact copy of Gnulib's template # =============================== # # Everything under this is an exact copy from the template # bootstrap.conf from Gnulib, it can readily be replaced with the # ending parts of an updated template. # Additional xgettext options to use. Use "\\\newline" to break lines. XGETTEXT_OPTIONS=$XGETTEXT_OPTIONS'\\\ --from-code=UTF-8\\\ --flag=asprintf:2:c-format --flag=vasprintf:2:c-format\\\ --flag=asnprintf:3:c-format --flag=vasnprintf:3:c-format\\\ --flag=wrapf:1:c-format\\\ ' # If "AM_GNU_GETTEXT(external" or "AM_GNU_GETTEXT([external]" # appears in configure.ac, exclude some unnecessary files. # Without grep's -E option (not portable enough, pre-configure), # the following test is ugly. Also, this depends on the existence # of configure.ac, not the obsolescent-named configure.in. But if # you're using this infrastructure, you should care about such things. gettext_external=0 grep '^[ ]*AM_GNU_GETTEXT(external\>' configure.ac > /dev/null && gettext_external=1 grep '^[ ]*AM_GNU_GETTEXT(\[external\]' configure.ac > /dev/null && gettext_external=1 if test $gettext_external = 1; then # Gettext supplies these files, but we don't need them since # we don't have an intl subdirectory. excluded_files=' m4/glibc2.m4 m4/intdiv0.m4 m4/lcmessage.m4 m4/lock.m4 m4/printf-posix.m4 m4/size_max.m4 m4/uintmax_t.m4 m4/ulonglong.m4 m4/visibility.m4 m4/xsize.m4 ' fi # Build prerequisites buildreq="\ autoconf 2.59 automake 1.9.6 git 1.5.5 tar - " gnuastro-0.2.33-8a3b/bootstrap0000755000175000017500000007556612722534072013107 00000000000000#! /bin/sh # Print a version string. scriptversion=2016-01-24.06; # UTC # Bootstrap this package from checked-out sources. # Copyright (C) 2003-2016 Free Software Foundation, Inc. # This program is free software: you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation, either version 3 of the License, or # (at your option) any later version. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # You should have received a copy of the GNU General Public License # along with this program. If not, see . # Originally written by Paul Eggert. The canonical version of this # script is maintained as build-aux/bootstrap in gnulib, however, to # be useful to your project, you should place a copy of it under # version control in the top-level directory of your project. The # intent is that all customization can be done with a bootstrap.conf # file also maintained in your version control; gnulib comes with a # template build-aux/bootstrap.conf to get you started. # Please report bugs or propose patches to bug-gnulib@gnu.org. nl=' ' # Ensure file names are sorted consistently across platforms. LC_ALL=C export LC_ALL # Ensure that CDPATH is not set. Otherwise, the output from cd # would cause trouble in at least one use below. (unset CDPATH) >/dev/null 2>&1 && unset CDPATH local_gl_dir=gl # Honor $PERL, but work even if there is none. PERL="${PERL-perl}" me=$0 usage() { cat <&2 } # warn_ WORD1... warn_ () { # If IFS does not start with ' ', set it and emit the warning in a subshell. case $IFS in ' '*) warnf_ '%s\n' "$*";; *) (IFS=' '; warn_ "$@");; esac } # die WORD1... die() { warn_ "$@"; exit 1; } # Configuration. # Name of the Makefile.am gnulib_mk=gnulib.mk # List of gnulib modules needed. gnulib_modules= # Any gnulib files needed that are not in modules. gnulib_files= : ${AUTOPOINT=autopoint} : ${AUTORECONF=autoreconf} # A function to be called right after gnulib-tool is run. # Override it via your own definition in bootstrap.conf. bootstrap_post_import_hook() { :; } # A function to be called after everything else in this script. # Override it via your own definition in bootstrap.conf. bootstrap_epilogue() { :; } # The command to download all .po files for a specified domain into # a specified directory. Fill in the first %s is the domain name, and # the second with the destination directory. Use rsync's -L and -r # options because the latest/%s directory and the .po files within are # all symlinks. po_download_command_format=\ "rsync --delete --exclude '*.s1' -Lrtvz \ 'translationproject.org::tp/latest/%s/' '%s'" # Fallback for downloading .po files (if rsync fails). po_download_command_format2=\ "wget --mirror -nd -q -np -A.po -P '%s' \ http://translationproject.org/latest/%s/" # Prefer a non-empty tarname (4th argument of AC_INIT if given), else # fall back to the package name (1st argument with munging) extract_package_name=' /^AC_INIT(\[*/{ s/// /^[^,]*,[^,]*,[^,]*,[ []*\([^][ ,)]\)/{ s//\1/ s/[],)].*// p q } s/[],)].*// s/^GNU // y/ABCDEFGHIJKLMNOPQRSTUVWXYZ/abcdefghijklmnopqrstuvwxyz/ s/[^abcdefghijklmnopqrstuvwxyz0123456789_]/-/g p } ' package=$(sed -n "$extract_package_name" configure.ac) \ || die 'cannot find package name in configure.ac' gnulib_name=lib$package build_aux=build-aux source_base=lib m4_base=m4 doc_base=doc tests_base=tests gnulib_extra_files='' # Additional gnulib-tool options to use. Use "\newline" to break lines. gnulib_tool_option_extras= # Other locale categories that need message catalogs. EXTRA_LOCALE_CATEGORIES= # Additional xgettext options to use. Use "\\\newline" to break lines. XGETTEXT_OPTIONS='\\\ --flag=_:1:pass-c-format\\\ --flag=N_:1:pass-c-format\\\ --flag=error:3:c-format --flag=error_at_line:5:c-format\\\ ' # Package bug report address and copyright holder for gettext files COPYRIGHT_HOLDER='Free Software Foundation, Inc.' MSGID_BUGS_ADDRESS=bug-$package@gnu.org # Files we don't want to import. excluded_files= # File that should exist in the top directory of a checked out hierarchy, # but not in a distribution tarball. checkout_only_file=README-hacking # Whether to use copies instead of symlinks. copy=false # Set this to '.cvsignore .gitignore' in bootstrap.conf if you want # those files to be generated in directories like lib/, m4/, and po/. # Or set it to 'auto' to make this script select which to use based # on which version control system (if any) is used in the source directory. vc_ignore=auto # Set this to true in bootstrap.conf to enable --bootstrap-sync by # default. bootstrap_sync=false # Use git to update gnulib sources use_git=true check_exists() { if test "$1" = "--verbose"; then ($2 --version /dev/null 2>&1 if test $? -ge 126; then # If not found, run with diagnostics as one may be # presented with env variables to set to find the right version ($2 --version /dev/null 2>&1 fi test $? -lt 126 } # find_tool ENVVAR NAMES... # ------------------------- # Search for a required program. Use the value of ENVVAR, if set, # otherwise find the first of the NAMES that can be run. # If found, set ENVVAR to the program name, die otherwise. # # FIXME: code duplication, see also gnu-web-doc-update. find_tool () { find_tool_envvar=$1 shift find_tool_names=$@ eval "find_tool_res=\$$find_tool_envvar" if test x"$find_tool_res" = x; then for i; do if check_exists $i; then find_tool_res=$i break fi done fi if test x"$find_tool_res" = x; then warn_ "one of these is required: $find_tool_names;" die "alternatively set $find_tool_envvar to a compatible tool" fi eval "$find_tool_envvar=\$find_tool_res" eval "export $find_tool_envvar" } # Override the default configuration, if necessary. # Make sure that bootstrap.conf is sourced from the current directory # if we were invoked as "sh bootstrap". case "$0" in */*) test -r "$0.conf" && . "$0.conf" ;; *) test -r "$0.conf" && . ./"$0.conf" ;; esac # Extra files from gnulib, which override files from other sources. test -z "${gnulib_extra_files}" && \ gnulib_extra_files=" build-aux/install-sh build-aux/mdate-sh build-aux/texinfo.tex build-aux/depcomp build-aux/config.guess build-aux/config.sub doc/INSTALL " if test "$vc_ignore" = auto; then vc_ignore= test -d .git && vc_ignore=.gitignore test -d CVS && vc_ignore="$vc_ignore .cvsignore" fi # Translate configuration into internal form. # Parse options. for option do case $option in --help) usage exit;; --gnulib-srcdir=*) GNULIB_SRCDIR=${option#--gnulib-srcdir=};; --skip-po) SKIP_PO=t;; --force) checkout_only_file=;; --copy) copy=true;; --bootstrap-sync) bootstrap_sync=true;; --no-bootstrap-sync) bootstrap_sync=false;; --no-git) use_git=false;; *) die "$option: unknown option";; esac done $use_git || test -d "$GNULIB_SRCDIR" \ || die "Error: --no-git requires --gnulib-srcdir" if test -n "$checkout_only_file" && test ! -r "$checkout_only_file"; then die "Bootstrapping from a non-checked-out distribution is risky." fi # Strip blank and comment lines to leave significant entries. gitignore_entries() { sed '/^#/d; /^$/d' "$@" } # If $STR is not already on a line by itself in $FILE, insert it at the start. # Entries are inserted at the start of the ignore list to ensure existing # entries starting with ! are not overridden. Such entries support # whitelisting exceptions after a more generic blacklist pattern. insert_if_absent() { file=$1 str=$2 test -f $file || touch $file test -r $file || die "Error: failed to read ignore file: $file" duplicate_entries=$(gitignore_entries $file | sort | uniq -d) if [ "$duplicate_entries" ] ; then die "Error: Duplicate entries in $file: " $duplicate_entries fi linesold=$(gitignore_entries $file | wc -l) linesnew=$( { echo "$str"; cat $file; } | gitignore_entries | sort -u | wc -l) if [ $linesold != $linesnew ] ; then { echo "$str" | cat - $file > $file.bak && mv $file.bak $file; } \ || die "insert_if_absent $file $str: failed" fi } # Adjust $PATTERN for $VC_IGNORE_FILE and insert it with # insert_if_absent. insert_vc_ignore() { vc_ignore_file="$1" pattern="$2" case $vc_ignore_file in *.gitignore) # A .gitignore entry that does not start with '/' applies # recursively to subdirectories, so prepend '/' to every # .gitignore entry. pattern=$(echo "$pattern" | sed s,^,/,);; esac insert_if_absent "$vc_ignore_file" "$pattern" } # Die if there is no AC_CONFIG_AUX_DIR($build_aux) line in configure.ac. found_aux_dir=no grep '^[ ]*AC_CONFIG_AUX_DIR(\['"$build_aux"'\])' configure.ac \ >/dev/null && found_aux_dir=yes grep '^[ ]*AC_CONFIG_AUX_DIR('"$build_aux"')' configure.ac \ >/dev/null && found_aux_dir=yes test $found_aux_dir = yes \ || die "configure.ac lacks 'AC_CONFIG_AUX_DIR([$build_aux])'; add it" # If $build_aux doesn't exist, create it now, otherwise some bits # below will malfunction. If creating it, also mark it as ignored. if test ! -d $build_aux; then mkdir $build_aux for dot_ig in x $vc_ignore; do test $dot_ig = x && continue insert_vc_ignore $dot_ig $build_aux done fi # Note this deviates from the version comparison in automake # in that it treats 1.5 < 1.5.0, and treats 1.4.4a < 1.4-p3a # but this should suffice as we won't be specifying old # version formats or redundant trailing .0 in bootstrap.conf. # If we did want full compatibility then we should probably # use m4_version_compare from autoconf. sort_ver() { # sort -V is not generally available ver1="$1" ver2="$2" # split on '.' and compare each component i=1 while : ; do p1=$(echo "$ver1" | cut -d. -f$i) p2=$(echo "$ver2" | cut -d. -f$i) if [ ! "$p1" ]; then echo "$1 $2" break elif [ ! "$p2" ]; then echo "$2 $1" break elif [ ! "$p1" = "$p2" ]; then if [ "$p1" -gt "$p2" ] 2>/dev/null; then # numeric comparison echo "$2 $1" elif [ "$p2" -gt "$p1" ] 2>/dev/null; then # numeric comparison echo "$1 $2" else # numeric, then lexicographic comparison lp=$(printf "$p1\n$p2\n" | LANG=C sort -n | tail -n1) if [ "$lp" = "$p2" ]; then echo "$1 $2" else echo "$2 $1" fi fi break fi i=$(($i+1)) done } get_version() { app=$1 $app --version >/dev/null 2>&1 || { $app --version; return 1; } $app --version 2>&1 | sed -n '# Move version to start of line. s/.*[v ]\([0-9]\)/\1/ # Skip lines that do not start with version. /^[0-9]/!d # Remove characters after the version. s/[^.a-z0-9-].*// # The first component must be digits only. s/^\([0-9]*\)[a-z-].*/\1/ #the following essentially does s/5.005/5.5/ s/\.0*\([1-9]\)/.\1/g p q' } check_versions() { ret=0 while read app req_ver; do # We only need libtoolize from the libtool package. if test "$app" = libtool; then app=libtoolize fi # Exempt git if --no-git is in effect. if test "$app" = git; then $use_git || continue fi # Honor $APP variables ($TAR, $AUTOCONF, etc.) appvar=$(echo $app | LC_ALL=C tr '[a-z]-' '[A-Z]_') test "$appvar" = TAR && appvar=AMTAR case $appvar in GZIP) ;; # Do not use $GZIP: it contains gzip options. PERL::*) ;; # Keep perl modules as-is *) eval "app=\${$appvar-$app}" ;; esac # Handle the still-experimental Automake-NG programs specially. # They remain named as the mainstream Automake programs ("automake", # and "aclocal") to avoid gratuitous incompatibilities with # pre-existing usages (by, say, autoreconf, or custom autogen.sh # scripts), but correctly identify themselves (as being part of # "GNU automake-ng") when asked their version. case $app in automake-ng|aclocal-ng) app=${app%-ng} ($app --version | grep '(GNU automake-ng)') >/dev/null 2>&1 || { warn_ "Error: '$app' not found or not from Automake-NG" ret=1 continue } ;; # Another check is for perl modules. These can be written as # e.g. perl::XML::XPath in case of XML::XPath module, etc. perl::*) # Extract module name app="${app#perl::}" if ! $PERL -m"$app" -e 'exit 0' >/dev/null 2>&1; then warn_ "Error: perl module '$app' not found" ret=1 fi continue ;; esac if [ "$req_ver" = "-" ]; then # Merely require app to exist; not all prereq apps are well-behaved # so we have to rely on $? rather than get_version. if ! check_exists --verbose $app; then warn_ "Error: '$app' not found" ret=1 fi else # Require app to produce a new enough version string. inst_ver=$(get_version $app) if [ ! "$inst_ver" ]; then warn_ "Error: '$app' not found" ret=1 else latest_ver=$(sort_ver $req_ver $inst_ver | cut -d' ' -f2) if [ ! "$latest_ver" = "$inst_ver" ]; then warnf_ '%s\n' \ "Error: '$app' version == $inst_ver is too old" \ " '$app' version >= $req_ver is required" ret=1 fi fi fi done return $ret } print_versions() { echo "Program Min_version" echo "----------------------" printf %s "$buildreq" echo "----------------------" # can't depend on column -t } # Find sha1sum, named gsha1sum on MacPorts, shasum on Mac OS X 10.6. # Also find the compatible sha1 utility on the BSDs if test x"$SKIP_PO" = x; then find_tool SHA1SUM sha1sum gsha1sum shasum sha1 fi use_libtool=0 # We'd like to use grep -E, to see if any of LT_INIT, # AC_PROG_LIBTOOL, AM_PROG_LIBTOOL is used in configure.ac, # but that's not portable enough (e.g., for Solaris). grep '^[ ]*A[CM]_PROG_LIBTOOL' configure.ac >/dev/null \ && use_libtool=1 grep '^[ ]*LT_INIT' configure.ac >/dev/null \ && use_libtool=1 if test $use_libtool = 1; then find_tool LIBTOOLIZE glibtoolize libtoolize fi # gnulib-tool requires at least automake and autoconf. # If either is not listed, add it (with minimum version) as a prerequisite. case $buildreq in *automake*) ;; *) buildreq="automake 1.9 $buildreq" ;; esac case $buildreq in *autoconf*) ;; *) buildreq="autoconf 2.59 $buildreq" ;; esac # When we can deduce that gnulib-tool will require patch, # and when patch is not already listed as a prerequisite, add it, too. if test -d "$local_gl_dir" \ && ! find "$local_gl_dir" -name '*.diff' -exec false {} +; then case $buildreq in *patch*) ;; *) buildreq="patch - $buildreq" ;; esac fi if ! printf "$buildreq" | check_versions; then echo >&2 if test -f README-prereq; then die "See README-prereq for how to get the prerequisite programs" else die "Please install the prerequisite programs" fi fi # Warn the user if autom4te appears to be broken; this causes known # issues with at least gettext 0.18.3. probe=$(echo 'm4_quote([hi])' | autom4te -l M4sugar -t 'm4_quote:$%' -) if test "x$probe" != xhi; then warn_ "WARNING: your autom4te wrapper eats stdin;" warn_ "if bootstrap fails, consider upgrading your autotools" fi echo "$0: Bootstrapping from checked-out $package sources..." # See if we can use gnulib's git-merge-changelog merge driver. if $use_git && test -d .git && check_exists git; then if git config merge.merge-changelog.driver >/dev/null ; then : elif check_exists git-merge-changelog; then echo "$0: initializing git-merge-changelog driver" git config merge.merge-changelog.name 'GNU-style ChangeLog merge driver' git config merge.merge-changelog.driver 'git-merge-changelog %O %A %B' else echo "$0: consider installing git-merge-changelog from gnulib" fi fi cleanup_gnulib() { status=$? rm -fr "$gnulib_path" exit $status } git_modules_config () { test -f .gitmodules && git config --file .gitmodules "$@" } if $use_git; then gnulib_path=$(git_modules_config submodule.gnulib.path) test -z "$gnulib_path" && gnulib_path=gnulib fi # Get gnulib files. Populate $GNULIB_SRCDIR, possibly updating a # submodule, for use in the rest of the script. case ${GNULIB_SRCDIR--} in -) # Note that $use_git is necessarily true in this case. if git_modules_config submodule.gnulib.url >/dev/null; then echo "$0: getting gnulib files..." git submodule init -- "$gnulib_path" || exit $? git submodule update -- "$gnulib_path" || exit $? elif [ ! -d "$gnulib_path" ]; then echo "$0: getting gnulib files..." trap cleanup_gnulib 1 2 13 15 shallow= git clone -h 2>&1 | grep -- --depth > /dev/null && shallow='--depth 2' git clone $shallow git://git.sv.gnu.org/gnulib "$gnulib_path" || cleanup_gnulib trap - 1 2 13 15 fi GNULIB_SRCDIR=$gnulib_path ;; *) # Use GNULIB_SRCDIR directly or as a reference. if $use_git && test -d "$GNULIB_SRCDIR"/.git && \ git_modules_config submodule.gnulib.url >/dev/null; then echo "$0: getting gnulib files..." if git submodule -h|grep -- --reference > /dev/null; then # Prefer the one-liner available in git 1.6.4 or newer. git submodule update --init --reference "$GNULIB_SRCDIR" \ "$gnulib_path" || exit $? else # This fallback allows at least git 1.5.5. if test -f "$gnulib_path"/gnulib-tool; then # Since file already exists, assume submodule init already complete. git submodule update -- "$gnulib_path" || exit $? else # Older git can't clone into an empty directory. rmdir "$gnulib_path" 2>/dev/null git clone --reference "$GNULIB_SRCDIR" \ "$(git_modules_config submodule.gnulib.url)" "$gnulib_path" \ && git submodule init -- "$gnulib_path" \ && git submodule update -- "$gnulib_path" \ || exit $? fi fi GNULIB_SRCDIR=$gnulib_path fi ;; esac # $GNULIB_SRCDIR now points to the version of gnulib to use, and # we no longer need to use git or $gnulib_path below here. if $bootstrap_sync; then cmp -s "$0" "$GNULIB_SRCDIR/build-aux/bootstrap" || { echo "$0: updating bootstrap and restarting..." case $(sh -c 'echo "$1"' -- a) in a) ignored=--;; *) ignored=ignored;; esac exec sh -c \ 'cp "$1" "$2" && shift && exec "${CONFIG_SHELL-/bin/sh}" "$@"' \ $ignored "$GNULIB_SRCDIR/build-aux/bootstrap" \ "$0" "$@" --no-bootstrap-sync } fi gnulib_tool=$GNULIB_SRCDIR/gnulib-tool <$gnulib_tool || exit $? # Get translations. download_po_files() { subdir=$1 domain=$2 echo "$me: getting translations into $subdir for $domain..." cmd=$(printf "$po_download_command_format" "$domain" "$subdir") eval "$cmd" && return # Fallback to HTTP. cmd=$(printf "$po_download_command_format2" "$subdir" "$domain") eval "$cmd" } # Mirror .po files to $po_dir/.reference and copy only the new # or modified ones into $po_dir. Also update $po_dir/LINGUAS. # Note po files that exist locally only are left in $po_dir but will # not be included in LINGUAS and hence will not be distributed. update_po_files() { # Directory containing primary .po files. # Overwrite them only when we're sure a .po file is new. po_dir=$1 domain=$2 # Mirror *.po files into this dir. # Usually contains *.s1 checksum files. ref_po_dir="$po_dir/.reference" test -d $ref_po_dir || mkdir $ref_po_dir || return download_po_files $ref_po_dir $domain \ && ls "$ref_po_dir"/*.po 2>/dev/null | sed 's|.*/||; s|\.po$||' > "$po_dir/LINGUAS" || return langs=$(cd $ref_po_dir && echo *.po | sed 's/\.po//g') test "$langs" = '*' && langs=x for po in $langs; do case $po in x) continue;; esac new_po="$ref_po_dir/$po.po" cksum_file="$ref_po_dir/$po.s1" if ! test -f "$cksum_file" || ! test -f "$po_dir/$po.po" || ! $SHA1SUM -c "$cksum_file" < "$new_po" > /dev/null 2>&1; then echo "$me: updated $po_dir/$po.po..." cp "$new_po" "$po_dir/$po.po" \ && $SHA1SUM < "$new_po" > "$cksum_file" || return fi done } case $SKIP_PO in '') if test -d po; then update_po_files po $package || exit fi if test -d runtime-po; then update_po_files runtime-po $package-runtime || exit fi;; esac symlink_to_dir() { src=$1/$2 dst=${3-$2} test -f "$src" && { # If the destination directory doesn't exist, create it. # This is required at least for "lib/uniwidth/cjk.h". dst_dir=$(dirname "$dst") if ! test -d "$dst_dir"; then mkdir -p "$dst_dir" # If we've just created a directory like lib/uniwidth, # tell version control system(s) it's ignorable. # FIXME: for now, this does only one level parent=$(dirname "$dst_dir") for dot_ig in x $vc_ignore; do test $dot_ig = x && continue ig=$parent/$dot_ig insert_vc_ignore $ig "${dst_dir##*/}" done fi if $copy; then { test ! -h "$dst" || { echo "$me: rm -f $dst" && rm -f "$dst" } } && test -f "$dst" && cmp -s "$src" "$dst" || { echo "$me: cp -fp $src $dst" && cp -fp "$src" "$dst" } else # Leave any existing symlink alone, if it already points to the source, # so that broken build tools that care about symlink times # aren't confused into doing unnecessary builds. Conversely, if the # existing symlink's time stamp is older than the source, make it afresh, # so that broken tools aren't confused into skipping needed builds. See # . test -h "$dst" && src_ls=$(ls -diL "$src" 2>/dev/null) && set $src_ls && src_i=$1 && dst_ls=$(ls -diL "$dst" 2>/dev/null) && set $dst_ls && dst_i=$1 && test "$src_i" = "$dst_i" && both_ls=$(ls -dt "$src" "$dst") && test "X$both_ls" = "X$dst$nl$src" || { dot_dots= case $src in /*) ;; *) case /$dst/ in *//* | */../* | */./* | /*/*/*/*/*/) die "invalid symlink calculation: $src -> $dst";; /*/*/*/*/) dot_dots=../../../;; /*/*/*/) dot_dots=../../;; /*/*/) dot_dots=../;; esac;; esac echo "$me: ln -fs $dot_dots$src $dst" && ln -fs "$dot_dots$src" "$dst" } fi } } version_controlled_file() { parent=$1 file=$2 if test -d .git; then git rm -n "$file" > /dev/null 2>&1 elif test -d .svn; then svn log -r HEAD "$file" > /dev/null 2>&1 elif test -d CVS; then grep -F "/${file##*/}/" "$parent/CVS/Entries" 2>/dev/null | grep '^/[^/]*/[0-9]' > /dev/null else warn_ "no version control for $file?" false fi } # NOTE: we have to be careful to run both autopoint and libtoolize # before gnulib-tool, since gnulib-tool is likely to provide newer # versions of files "installed" by these two programs. # Then, *after* gnulib-tool (see below), we have to be careful to # run autoreconf in such a way that it does not run either of these # two just-pre-run programs. # Import from gettext. with_gettext=yes grep '^[ ]*AM_GNU_GETTEXT_VERSION(' configure.ac >/dev/null || \ with_gettext=no if test $with_gettext = yes || test $use_libtool = 1; then tempbase=.bootstrap$$ trap "rm -f $tempbase.0 $tempbase.1" 1 2 13 15 > $tempbase.0 > $tempbase.1 && find . ! -type d -print | sort > $tempbase.0 || exit if test $with_gettext = yes; then # Released autopoint has the tendency to install macros that have been # obsoleted in current gnulib, so run this before gnulib-tool. echo "$0: $AUTOPOINT --force" $AUTOPOINT --force || exit fi # Autoreconf runs aclocal before libtoolize, which causes spurious # warnings if the initial aclocal is confused by the libtoolized # (or worse out-of-date) macro directory. # libtoolize 1.9b added the --install option; but we support back # to libtoolize 1.5.22, where the install action was default. if test $use_libtool = 1; then install= case $($LIBTOOLIZE --help) in *--install*) install=--install ;; esac echo "running: $LIBTOOLIZE $install --copy" $LIBTOOLIZE $install --copy fi find . ! -type d -print | sort >$tempbase.1 old_IFS=$IFS IFS=$nl for file in $(comm -13 $tempbase.0 $tempbase.1); do IFS=$old_IFS parent=${file%/*} version_controlled_file "$parent" "$file" || { for dot_ig in x $vc_ignore; do test $dot_ig = x && continue ig=$parent/$dot_ig insert_vc_ignore "$ig" "${file##*/}" done } done IFS=$old_IFS rm -f $tempbase.0 $tempbase.1 trap - 1 2 13 15 fi # Import from gnulib. gnulib_tool_options="\ --import\ --no-changelog\ --aux-dir $build_aux\ --doc-base $doc_base\ --lib $gnulib_name\ --m4-base $m4_base/\ --source-base $source_base/\ --tests-base $tests_base\ --local-dir $local_gl_dir\ $gnulib_tool_option_extras\ " if test $use_libtool = 1; then case "$gnulib_tool_options " in *' --libtool '*) ;; *) gnulib_tool_options="$gnulib_tool_options --libtool" ;; esac fi echo "$0: $gnulib_tool $gnulib_tool_options --import ..." $gnulib_tool $gnulib_tool_options --import $gnulib_modules \ || die "gnulib-tool failed" for file in $gnulib_files; do symlink_to_dir "$GNULIB_SRCDIR" $file \ || die "failed to symlink $file" done bootstrap_post_import_hook \ || die "bootstrap_post_import_hook failed" # Remove any dangling symlink matching "*.m4" or "*.[ch]" in some # gnulib-populated directories. Such .m4 files would cause aclocal to fail. # The following requires GNU find 4.2.3 or newer. Considering the usual # portability constraints of this script, that may seem a very demanding # requirement, but it should be ok. Ignore any failure, which is fine, # since this is only a convenience to help developers avoid the relatively # unusual case in which a symlinked-to .m4 file is git-removed from gnulib # between successive runs of this script. find "$m4_base" "$source_base" \ -depth \( -name '*.m4' -o -name '*.[ch]' \) \ -type l -xtype l -delete > /dev/null 2>&1 # Invoke autoreconf with --force --install to ensure upgrades of tools # such as ylwrap. AUTORECONFFLAGS="--verbose --install --force -I $m4_base $ACLOCAL_FLAGS" # Some systems (RHEL 5) are using ancient autotools, for which the # --no-recursive option had not been invented. Detect that lack and # omit the option when it's not supported. FIXME in 2017: remove this # hack when RHEL 5 autotools are updated, or when they become irrelevant. case $($AUTORECONF --help) in *--no-recursive*) AUTORECONFFLAGS="$AUTORECONFFLAGS --no-recursive";; esac # Tell autoreconf not to invoke autopoint or libtoolize; they were run above. echo "running: AUTOPOINT=true LIBTOOLIZE=true $AUTORECONF $AUTORECONFFLAGS" AUTOPOINT=true LIBTOOLIZE=true $AUTORECONF $AUTORECONFFLAGS \ || die "autoreconf failed" # Get some extra files from gnulib, overriding existing files. for file in $gnulib_extra_files; do case $file in */INSTALL) dst=INSTALL;; build-aux/*) dst=$build_aux/${file#build-aux/};; *) dst=$file;; esac symlink_to_dir "$GNULIB_SRCDIR" $file $dst \ || die "failed to symlink $file" done if test $with_gettext = yes; then # Create gettext configuration. echo "$0: Creating po/Makevars from po/Makevars.template ..." rm -f po/Makevars sed ' /^EXTRA_LOCALE_CATEGORIES *=/s/=.*/= '"$EXTRA_LOCALE_CATEGORIES"'/ /^COPYRIGHT_HOLDER *=/s/=.*/= '"$COPYRIGHT_HOLDER"'/ /^MSGID_BUGS_ADDRESS *=/s|=.*|= '"$MSGID_BUGS_ADDRESS"'| /^XGETTEXT_OPTIONS *=/{ s/$/ \\/ a\ '"$XGETTEXT_OPTIONS"' $${end_of_xgettext_options+} } ' po/Makevars.template >po/Makevars \ || die 'cannot generate po/Makevars' # If the 'gettext' module is in use, grab the latest Makefile.in.in. # If only the 'gettext-h' module is in use, assume autopoint already # put the correct version of this file into place. case $gnulib_modules in *gettext-h*) ;; *gettext*) cp $GNULIB_SRCDIR/build-aux/po/Makefile.in.in po/Makefile.in.in \ || die "cannot create po/Makefile.in.in" ;; esac if test -d runtime-po; then # Similarly for runtime-po/Makevars, but not quite the same. rm -f runtime-po/Makevars sed ' /^DOMAIN *=.*/s/=.*/= '"$package"'-runtime/ /^subdir *=.*/s/=.*/= runtime-po/ /^MSGID_BUGS_ADDRESS *=/s/=.*/= bug-'"$package"'@gnu.org/ /^XGETTEXT_OPTIONS *=/{ s/$/ \\/ a\ '"$XGETTEXT_OPTIONS_RUNTIME"' $${end_of_xgettext_options+} } ' po/Makevars.template >runtime-po/Makevars \ || die 'cannot generate runtime-po/Makevars' # Copy identical files from po to runtime-po. (cd po && cp -p Makefile.in.in *-quot *.header *.sed *.sin ../runtime-po) fi fi bootstrap_epilogue echo "$0: done. Now you can run './configure'." # Local variables: # eval: (add-hook 'write-file-hooks 'time-stamp) # time-stamp-start: "scriptversion=" # time-stamp-format: "%:y-%02m-%02d.%02H" # time-stamp-time-zone: "UTC0" # time-stamp-end: "; # UTC" # End: gnuastro-0.2.33-8a3b/THANKS0000644000175000017500000000352713003417675012045 00000000000000GNU Astronomy Utilities Acknowledgments ======================================= The following people and institutions who contributed to Gnuastro indirectly (not by actually submitting code) are listed here. For the list of Gnuastro code/documentation authors (people who have contributed actual code/text as commits in the version controlled history of Gnuastro), please see the `AUTHORS' file in the same directory. People ------ The following people provided valuable feedback (suggestions, ideas) to the authors of Gnuastro. We hereby gratefully acknowledge their help and support in Gnuastro. The list is ordered alphabetically. Karl Berry karl@gnu.org Roland Bacon roland.bacon@univ-lyon1.fr Antonio Diaz Diaz antonio@gnu.org Takashi Ichikawa ichikawa@astr.tohoku.ac.jp Brandon Invergo brandon@gnu.org Mohammad-Reza Khellat moha.khe@gmail.com Alan Lefor alefor@astr.tohoku.ac.jp Francesco Montanari francesco.montanari@openmailbox.org Yahya Sefidbakht y.sefidbakht@gmail.com Richard Stallman rms@gnu.org Ole Streicher olebole@debian.org Institutions ------------ GNU Astronomy Utilities (Gnuastro) has greatly benefited from the following institutions. These institutions have either funded, supported and most importantly provided a productive environment for the developers of Gnuastro. The list is in chronological order. Ministry of education, culture, sports, science and technology, Japan. Tohoku University, Sendai, Japan. University of Salento, Lecce, Italy. Centre de Recherche Astrophysique de Lyon, France Centre national de la recherche scientifique, Francegnuastro-0.2.33-8a3b/NEWS0000644000175000017500000003117413003237624011622 00000000000000GNU Astronomy Utilities NEWS -*- outline -*- * Noteworthy changes in release 0.2.28 (library 1.0.0) (2016-10-23) [alpha] ** Bug fixes Using `%zu' to print `size_t' variables for clean build on 32-bit systems. Crash in Table for some operating systems due to memory is now fixed (bug #49347). Table's man-page is now created and installed (bug #49418). Fixes in the documentation (sr #109170, bug #49419). ** New programs, functions, or macros `gal_wcs_pixel_scale_deg' Returns the pixel scale of the input WCS structure in degrees. `gal_wcs_angular_distance_deg' This has replaced `gal_wcs_angular_distance'. That function would take the angles in radians and also return its value in radians. Radians are very inconvenient and uncommon in celestial coordinates, so its input and output was modified to accept angles in degrees and also return the angular distance in degrees. `gnuastro/git.h' New header for wrappers on the Git library. `gal_git_describe' Bascially a wrapper on Git's describe functions to return the string for easy inclusion. `gal_fits_datatype_size Return the size (in bytes) of the given datatype. `GAL_GNUASTRO_HAVE_PTHREAD_BARRIER' This is a new name for the old `GAL_GNUASTRO_PTHREAD_BARRIER' to conform better with other such marcos. `GAL_GNUASTRO_HAVE_LIBGIT2' Has a value of 1 if the host system has the Git library (`libgit2'). ** Removed programs, functions, macros `gal_wcs_angular_distance' See the explanation above for `gal_wcs_angular_distance_deg'. `GAL_GNUASTRO_PTHREAD_BARRIER' See the explanation above for `GAL_GNUASTRO_HAVE_PTHREAD_BARRIER'. ** New features ImageWarp can now align the image with the celestial coordiates using the `--align' option. ImageWarp can now warp without an input matrix, using the following options: `--shear', `--flip', `--project', `--rotate', `--scale', `--translate'. Any number of these transformations (along with the `--align' option) can be called at runtime and they will be applied in the same order to create one warping matrix. By default the FITS coordinates will also be corrected. ** Changes in behavior When a 2 by 2 matrix is given to ImageWarp, the FITS pixel positions (which define the center of a pixel as an integer) are automatically implemented internally, see "Invoking ImageWarp" in the manual for more. `gal_fits_write_keys_version' will now also write the Git commit description when the Git library is installed on the host system. * Noteworthy changes in release 0.2 (library 0.0.0) (2016-10-03) [stable] ** Bug fixes Linker errors on some operating systems have been fixed (bug #48076). Several memory allocation, checks or redundancies have been fixed: bugs #48453, #48516, #48603, #48611, #48571, #48650, #48657, #48692, #48770, #47866, #48899, #49049, #49007. ImageCrop no longer crashes with very long output file names (bugs #46241 and #45380). ** New programs or headers Table: a new utility to read and write FITS binary and ASCII tables. It can also print the column information or select columns using regular expressions (task #13579). Shared libraries and headers are now installed. The libraries can be used in C and C++ programs. This release includes the following headers: `gnuastro.h', `array.h', `box.h', `fits.h', `linkedlist.h', `mesh.h', `polygon.h', `qsort.h', `spatialconvolve.h', `statistics.h', `threads.h', `wcs.h', `txtarray.h' (task #13765). Gnuastro now comes with a script in its top source directory (`tmpfs-config-make') to configure and build it in the tmpfs (on the RAM), for those systems that have it. See the new "Configure and build in RAM" section in the book for more (task #14100). ** New features MakeProfiles also accepts WCS positions (task #13566). Flat profiles in MakeProfiles can be given a profile specific value. The new `--mforflatpix' option MakeProfile will use the value in the magnitude column as a fixed value for each pixel. This can be very useful in defining a mask, or creating segmentation maps or labeled images (task #14115). MakeProfiles can now use input image as canvas. Instead of specifying the WSC and image size paramteres manually. With the new `--inputascanvas' option, MakeProfiles will get this information (along with blank pixels) from an already existing image (task #14116). Type of output in MakeProfiles and Arithmetic can be specified with the `--type' option. Magnitude error column in MakeCatalog with the `--magnitudeerr' option. Arithmetic now has new conditional (task #13870) and logical operators (task #14153) along with an operator for actions only when conditions are true: `where'. The new `isblank' operator will also enable you to select blank, or masked, pixels (task #14146). The `--noerodequant' in NoiseChisel enables it to detect small and sharper profiles by disabling erosion on pixels above a certain quantile (task #14139). MakeCatalog can also calculate the upper limit magnitude for each given object in the image by randomly positioning the object's footprint over undetected regions of the image (task #14167). The source tarball is now also distributed with Lzip for a much better compression ratio and more robust archival file format. ** Changes in behavior The two MakeProfiles options `--setconsttonan', `--setconsttomin' have been removed (see `--mforflatpix' above for their alternative). MakeCatalog makes clump catalog only when asked (when the `WCLUMPS' header exists in the objects HDU). This can be very useful in cases like aperture photometry, when the object labels are not generated by NoiseChisel and so a clump image doesn't exist (task #14122). Default cosmological parameters in CosmiCalculator set to Plank 2015 results: A&A (2016), 594, A13 (arXiv 1502.01589). The `--envseed' option (to read random number generator type and seed from the environment) to MakeProfiles and MakeNoise can also be given in the configuration files. * Noteworthy changes in release 0.1 (2016-05-30) [stable] ** Bug fixes MakeCatalog's problem in checking the sizes of all input images is now fixed. NoiseChisel's problem with reading the `--kernel' option is now corrected (bug #46750). lib/mesh.c's problem in correctly calculating the mesh sizes was corrected (bug #47611). `make check' will not look into system utility configuration files. In the previous release, if Gnuastro was already installed, the configuration files already present on the system would also be read. Now only configuration files in the tested package are used (bug #47833). Ghostscript's version is now checked at configure time after its existence. ConvertType uses the `-dPDFFitPage' option to Ghostscript which was introduced in version 9.10, so older versions would pass configure but at `make check' time, the PDF test would fail. Now this test is skipped (bug #47868). Most tests would fail when `make check -jN' was run (to do the checks on N threads). A dependency structure has now been defined to fix this problem and greatly speed up the testing process (bug #47957). ** New utilities Arithmetic: For arithmetic operations on the pixels of input images. With this utility, it is now possible to add multiple images with each other, or easily calculate a median image. It as a large set of other arithmetic operations and some functions which can be done on the input image(s). An unlimited number of input images can be given, the images will only be loaded when necessary and will be freed as soon as they are no longer necessary. CosmicCalculator: For doing cosmological calculations at a given redshift. ** New features All the utilities that would produce a log file now have a `--nolog' option to avoid printing a log file. The tiled image compression convention (.fits.fz, created with `fpack') files can now be used as input in the utilities. ImageCrop can now also crop a polygon from the input image. The polygon vertices can be given in the world or image coordinates. The simple `--polygon' option will keep the insides of the polygon while the `--outpolygon' will keep the outside of the polygon. ImageCrop and ImageWarp can now read the WCS information of a FITS header from a specific region with the `--hstartwcs' and `--hendwcs'. In some older FITS images, when the WCS distortions were not as standardized as now, there were cases which would confuse WCSLIB. NoiseChisel can now save the grown clumps image instead of the original clumps image in the output with the `--grownclumps' option. Convolve can now do deconvolution with the `--makekernel' option. MakeProfiles now has a `--setconsttonan' option which will fill the contant profiles with a NaN (blank) value, not a number, allowing the creations of elliptical masked regions for example. Header can now import a keyword directly from a string with the `--asis' option. MakeCatalog can now output the geometric (average position independent of pixel flux value) positions of the objects too. MakeCatalog can now produce the object's elliptical parameters (for example semi-major axis, semi-minor axis, and position angle). This can also be done both in standard flux weighted and geometric methods too. MakeCatalog now has a `--threshold' function to only use pixels above a given threshold in each object or clump. This is useful to avoid diffuse regions in calculations. MakeCatalog now has a `--noriverbrightness' option. With this option it is possible to calculate the clump flux without subtracting the river pixels on its circumference. The number of CPU threads is no longer a configuration option, it is now determined at runtime for each program. Therefore it is now easily possible to built Gnuastro on one system to use on another (commonly done in the GNU/Linux package managers). Therefore ./configure no longer has a `--with-numthreads' option. Every commit in Gnuastro's history (after implementing this feature) can now be given a unique version number. Since the version number is printed in possible outputs, this feature can help reproducibility, even when the an official/stable release isn't used. The AUTHORS file is now automatically generated from the version controlled history. Also all the authors that have contributed to Gnuastro are included in the second (copyright) page of the PDF book. All the bootstrapped directories are now moved with a new `bootstrapped' directory in the top source directory. This significantly cleans up this directory, allowing users to more easily find the hand-written Gnuastro source files they like. A `bug-gnuastro' Info page was created so users can easily go to that page for information on how to submit bug reports. It is accessible on the command line with the command `info bug-gnuastro'. ** Changes in behavior The separate utilities no longer have a separate version number. With the introduction of unofficial version numbers generated from each commit in Gnuastro's history, the utility version numbers would cause confusion. MakeProfiles will now add a suffix to the individual images and put them in the output directory if specified. NoiseChisel and MakeCatalog now use the median mesh standard deviation to define the over-all depth of the image. Previously they used the maximum value (or the least depth). NoiseChisel no longer outputs a sky subtracted image. This job can now be done with the new Arithmetic utility. NoiseChisel's `--segsnhistnbins' option was renamed to `--clumpsnhistnbins'. ** Improvements NoiseChisel's default quantiles were changed to 0.95 from 0.99. Since the old value was too severe. NoiseChisel's S/N thresholds are now found from the distribution of pseudo-detections and clumps from the full image, not within each large mesh. This was done to increase the accuracy of the S/N threshold. There were commonly not enough points in large mesh sizes and this would add scatter. With ImageCrop's polygon capabilities, it is now easily possible to cut out the region that has uniform noise properties (depth and correlated noise). Therefore the old `--checkdetectionsn' and `checkclumpsn' options are no longer present. When building from the version controlled source, the whole bootstrapping process is done with one script. In the previous version, all the separate operations should have been done by hand (as instructed in the old manual). All the build steps now report what was done and suggest the next step. This feature can be disabled with the `--disable-guide-message' at configure time. gnuastro-0.2.33-8a3b/INSTALL0000644000175000017500000003661412744162475012174 00000000000000Installation Instructions ************************* Copyright (C) 1994-1996, 1999-2002, 2004-2016 Free Software Foundation, Inc. Copying and distribution of this file, with or without modification, are permitted in any medium without royalty provided the copyright notice and this notice are preserved. This file is offered as-is, without warranty of any kind. Basic Installation ================== Briefly, the shell command './configure && make && make install' should configure, build, and install this package. The following more-detailed instructions are generic; see the 'README' file for instructions specific to this package. Some packages provide this 'INSTALL' file but do not implement all of the features documented below. The lack of an optional feature in a given package is not necessarily a bug. More recommendations for GNU packages can be found in *note Makefile Conventions: (standards)Makefile Conventions. The 'configure' shell script attempts to guess correct values for various system-dependent variables used during compilation. It uses those values to create a 'Makefile' in each directory of the package. It may also create one or more '.h' files containing system-dependent definitions. Finally, it creates a shell script 'config.status' that you can run in the future to recreate the current configuration, and a file 'config.log' containing compiler output (useful mainly for debugging 'configure'). It can also use an optional file (typically called 'config.cache' and enabled with '--cache-file=config.cache' or simply '-C') that saves the results of its tests to speed up reconfiguring. Caching is disabled by default to prevent problems with accidental use of stale cache files. If you need to do unusual things to compile the package, please try to figure out how 'configure' could check whether to do them, and mail diffs or instructions to the address given in the 'README' so they can be considered for the next release. If you are using the cache, and at some point 'config.cache' contains results you don't want to keep, you may remove or edit it. The file 'configure.ac' (or 'configure.in') is used to create 'configure' by a program called 'autoconf'. You need 'configure.ac' if you want to change it or regenerate 'configure' using a newer version of 'autoconf'. The simplest way to compile this package is: 1. 'cd' to the directory containing the package's source code and type './configure' to configure the package for your system. Running 'configure' might take a while. While running, it prints some messages telling which features it is checking for. 2. Type 'make' to compile the package. 3. Optionally, type 'make check' to run any self-tests that come with the package, generally using the just-built uninstalled binaries. 4. Type 'make install' to install the programs and any data files and documentation. When installing into a prefix owned by root, it is recommended that the package be configured and built as a regular user, and only the 'make install' phase executed with root privileges. 5. Optionally, type 'make installcheck' to repeat any self-tests, but this time using the binaries in their final installed location. This target does not install anything. Running this target as a regular user, particularly if the prior 'make install' required root privileges, verifies that the installation completed correctly. 6. You can remove the program binaries and object files from the source code directory by typing 'make clean'. 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Run './configure --help' for details on some of the pertinent environment variables. You can give 'configure' initial values for configuration parameters by setting variables in the command line or in the environment. Here is an example: ./configure CC=c99 CFLAGS=-g LIBS=-lposix *Note Defining Variables::, for more details. Compiling For Multiple Architectures ==================================== You can compile the package for more than one kind of computer at the same time, by placing the object files for each architecture in their own directory. To do this, you can use GNU 'make'. 'cd' to the directory where you want the object files and executables to go and run the 'configure' script. 'configure' automatically checks for the source code in the directory that 'configure' is in and in '..'. This is known as a "VPATH" build. With a non-GNU 'make', it is safer to compile the package for one architecture at a time in the source code directory. After you have installed the package for one architecture, use 'make distclean' before reconfiguring for another architecture. On MacOS X 10.5 and later systems, you can create libraries and executables that work on multiple system types--known as "fat" or "universal" binaries--by specifying multiple '-arch' options to the compiler but only a single '-arch' option to the preprocessor. Like this: ./configure CC="gcc -arch i386 -arch x86_64 -arch ppc -arch ppc64" \ CXX="g++ -arch i386 -arch x86_64 -arch ppc -arch ppc64" \ CPP="gcc -E" CXXCPP="g++ -E" This is not guaranteed to produce working output in all cases, you may have to build one architecture at a time and combine the results using the 'lipo' tool if you have problems. 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For these packages, running './configure --enable-silent-rules' sets the default to minimal output, which can be overridden with 'make V=1'; while running './configure --disable-silent-rules' sets the default to verbose, which can be overridden with 'make V=0'. Particular systems ================== On HP-UX, the default C compiler is not ANSI C compatible. If GNU CC is not installed, it is recommended to use the following options in order to use an ANSI C compiler: ./configure CC="cc -Ae -D_XOPEN_SOURCE=500" and if that doesn't work, install pre-built binaries of GCC for HP-UX. HP-UX 'make' updates targets which have the same time stamps as their prerequisites, which makes it generally unusable when shipped generated files such as 'configure' are involved. Use GNU 'make' instead. On OSF/1 a.k.a. Tru64, some versions of the default C compiler cannot parse its '' header file. The option '-nodtk' can be used as a workaround. If GNU CC is not installed, it is therefore recommended to try ./configure CC="cc" and if that doesn't work, try ./configure CC="cc -nodtk" On Solaris, don't put '/usr/ucb' early in your 'PATH'. This directory contains several dysfunctional programs; working variants of these programs are available in '/usr/bin'. So, if you need '/usr/ucb' in your 'PATH', put it _after_ '/usr/bin'. On Haiku, software installed for all users goes in '/boot/common', not '/usr/local'. It is recommended to use the following options: ./configure --prefix=/boot/common Specifying the System Type ========================== There may be some features 'configure' cannot figure out automatically, but needs to determine by the type of machine the package will run on. Usually, assuming the package is built to be run on the _same_ architectures, 'configure' can figure that out, but if it prints a message saying it cannot guess the machine type, give it the '--build=TYPE' option. TYPE can either be a short name for the system type, such as 'sun4', or a canonical name which has the form: CPU-COMPANY-SYSTEM where SYSTEM can have one of these forms: OS KERNEL-OS See the file 'config.sub' for the possible values of each field. If 'config.sub' isn't included in this package, then this package doesn't need to know the machine type. If you are _building_ compiler tools for cross-compiling, you should use the option '--target=TYPE' to select the type of system they will produce code for. If you want to _use_ a cross compiler, that generates code for a platform different from the build platform, you should specify the "host" platform (i.e., that on which the generated programs will eventually be run) with '--host=TYPE'. Sharing Defaults ================ If you want to set default values for 'configure' scripts to share, you can create a site shell script called 'config.site' that gives default values for variables like 'CC', 'cache_file', and 'prefix'. 'configure' looks for 'PREFIX/share/config.site' if it exists, then 'PREFIX/etc/config.site' if it exists. Or, you can set the 'CONFIG_SITE' environment variable to the location of the site script. A warning: not all 'configure' scripts look for a site script. Defining Variables ================== Variables not defined in a site shell script can be set in the environment passed to 'configure'. However, some packages may run configure again during the build, and the customized values of these variables may be lost. In order to avoid this problem, you should set them in the 'configure' command line, using 'VAR=value'. For example: ./configure CC=/usr/local2/bin/gcc causes the specified 'gcc' to be used as the C compiler (unless it is overridden in the site shell script). Unfortunately, this technique does not work for 'CONFIG_SHELL' due to an Autoconf limitation. Until the limitation is lifted, you can use this workaround: CONFIG_SHELL=/bin/bash ./configure CONFIG_SHELL=/bin/bash 'configure' Invocation ====================== 'configure' recognizes the following options to control how it operates. '--help' '-h' Print a summary of all of the options to 'configure', and exit. '--help=short' '--help=recursive' Print a summary of the options unique to this package's 'configure', and exit. The 'short' variant lists options used only in the top level, while the 'recursive' variant lists options also present in any nested packages. '--version' '-V' Print the version of Autoconf used to generate the 'configure' script, and exit. '--cache-file=FILE' Enable the cache: use and save the results of the tests in FILE, traditionally 'config.cache'. FILE defaults to '/dev/null' to disable caching. '--config-cache' '-C' Alias for '--cache-file=config.cache'. '--quiet' '--silent' '-q' Do not print messages saying which checks are being made. To suppress all normal output, redirect it to '/dev/null' (any error messages will still be shown). '--srcdir=DIR' Look for the package's source code in directory DIR. Usually 'configure' can determine that directory automatically. '--prefix=DIR' Use DIR as the installation prefix. *note Installation Names:: for more details, including other options available for fine-tuning the installation locations. '--no-create' '-n' Run the configure checks, but stop before creating any output files. 'configure' also accepts some other, not widely useful, options. Run 'configure --help' for more details. gnuastro-0.2.33-8a3b/ChangeLog0000644000175000017500000012014312771240103012665 000000000000002016-05-27 Mohammad Akhlaghi Following the discussions in task #13779, the ChangeLog has not been updated since 2015-11-05 (previous log). Instead, the commit messages are very descriptive. Git's blame tool can be used to check the history of any part of the code very effectively. Gnulib has scripts to generate a ChangeLog from the commit history so building this file automatically is possible and will be implemented (task #14007). Once this ChangeLog is automatically generated, it will be removed from the version controlled source. Until then this file will remain unchanged. There is also a discussion for adopting the ChangeLog format in the commit messages in task #14008. * ChangeLog: no longer updated. 2015-11-05 Mohammad Akhlaghi * doc/gnuastro.texi (Why C): Clarified explanations. 2015-11-04 Mosè Giordano * .gitignore: Add new regexps to the list of ignored files. * doc/gnuastro.texi (Arguments): Mention new accepted extension. * lib/fitsarrayvv.c (nameisfits): Add "fits.fz" to the list of accepted extensions. Fixes task#13767. (nameisfitssuffix): Ditto. 2015-10-18 Mosè Giordano * bin/imgcrop/imgcrop.c (imgcrop): Do not use modefunction to set the function, run the functions manually instead. Fixes bug#45380. 2015-10-16 Mosè Giordano * ./*: Change in many files the name of the package from "gnuastro" to "Gnuastro". Fixes bug#46212. * doc/forwebpage.sh: Use canonical path for bash shell. * doc/plotbin/conversions.sh: Ditto. 2015-10-02 Mohammad Akhlaghi * bin/noisechisel/noisechisel.c (makeoutput): Added a "raw" term in the comments of the noise statistics so emphasize that this is from the raw mesh grid and not the interpolated and smoothed grid. * bin/mkcatalog/mkcatalog.c (makeoutput): As explained below. * doc/gnuastro.texi (Depth and limiting magnitude): Changed the sigma which representes depth from the maximum to the median. The maximum has a strong scatter and even one mesh can completely push to unreasonable values. But the median is not affected by such minor mesh variations, so it is a more robust measure of the dispersion. 2015-10-01 Mohammad Akhlaghi * bin/imgcrop/ui.c (checkifset): Removed the hstartwcs and hendwcs options as mandatory arguments. * lib/fitsarrayvv.c (readfitswcs): Now applies the hstartwcs and hendwcs options. * include/fitsarrayvv.h: readfitswcs now takes the hstartwcs and hendwcs values as arguments. This was done so all programs could take in these options. 2015-09-23 Mohammad Akhlaghi * doc/gnuastro.texi (Depth and limiting magnitude): Updated explanations in for the depth and limiting magnitude to be more realistic. * bin/mkcatalog/mkcatalog.c (makeoutput): Removed the limiting magnitude calculation that was previously defined since it's physical meaning is very unclear (it was mainly put as a test). Also changed the surface brightness limit to a per-pixel basis (independent of the projected area of the pixel) as explained in the manual. 2015-09-17 Mohammad Akhlaghi * bin/mkprof/mkprof.c (mkprof): Only print a log file if the `--nolog' option is not called. * bin/imgcrop/imgcrop.c (imgcrop): Only print a log file if the `--nolog' option is not called. * bin/mkprof/main.h (mkprofparams): Removed the p->dir0file1 parameter from the main structure. * tests/mkprof/mosaic1.sh: Corrected the name of the first output for the new individual name configuration (where the output file name is suffixed to the row number). * bin/mkprof/ui.c (sanitycheck): Now everything based on the situation the basic information for the next steps is set here. * bin/mkprof/mkprof.c (saveindividual): Removed the name checking here. All the necessary information is now set in ui.c. 2015-09-13 Mohammad Akhlaghi * bin/imgwarp/imgwarp.c (imgwarponthread): Now calculates the fraction of area that is blank (NaN) and if that fraction is larger than a user defined value, then the output pixel will be blank. Before the blank fraction was ignored. * bin/imgstat/imgstat.c (reportsimplestats): Now uses the value to the `--mirrordist' option instead of the fixed value of 1.5. (reportsimplestats): Report the `NOT ACCURATE' warning in a separate line to make reading by AWK easier, also removed comma between outputs for the same reason. * bin/*/ui.c (readconfig): Now uses macros for common options. (printvalues): Similarly uses macros for common options. * lib/statistics.c (sigmaclip_converge): Removed commas between the outputs to make reading by AWK easier. (sigmaclip_certainnum): Similar to above. * include/fixedstringmacros.h (GNUASTROBIBTEX): New name from ASTRUTILSBIBTEX. Also the content was updated to the full ADS BibTeX output after the paper was published. * include/configfiles.h (CHECKSETCONFIG): Now checks for the version of the program and also has a more cleaner/readable path for reading/writing to the user configuration directory and reading from the system configuration directory. 2015-08-16 Mohammad Akhlaghi * bin/noisechisel/thresh.c (snthresh): The check on the number of objects in finding the S/N threshold is now done before sorting the S/N table. * bin/convolve/convolve.c (removepaddingcorrectroundoff): When the maximum radius is smaller than the input images, then the final kernel will be shrinked to have no only-zero column or row. 2015-08-05 Mohammad Akhlaghi * bin/convolve/convolve.c (frequencyconvolve): Divide the arrays when the kernel should be made, multiply them when convolution is to be done. (frequencyconvolve): When in deconvolution mode, it will go to another function to make the final product. 2015-07-31 Mohammad Akhlaghi * bin/convolve/convolve.c (makepaddedcomplex): Added a check to make the padded image size an even number in both dimensions by adding one pixel if it is odd. This was done because FFT operations work much faster on even sized arrays. 2015-07-22 Mohammad Akhlaghi * bin/noisechisel/thresh.c (snthresh): Had mistakenly used `p->detquant', for both detection and segmentation! This is now corrected. * bin/mkcatalog/mkcatalog.c (secondpass): Sets the river flux to Sky for when the grown clumps are used, see the explanation bellow. * bin/mkcatalog/columns.c (brightnessmag): Corrected the definition of brightness. It was incorrectly dividing the total brightness by the area when the user asked for brightness. (sncol): Can now work accurately when grown clumps are also included. In a grown clump image, full detections that aren't harmed by deblending are are fully labeled. So there is no river pixels there and the S/N equations had to incorporate this. 2015-07-18 Mohammad Akhlaghi * bin/noisechisel/segmentation.c (nextavailablelabel): Now accounts for the `--grownclumps' option. * bin/noisechisel/args.h (options): Corrected the type of output for `--gthresh'. I had forgot to include any for it! 2015-07-17 Mohammad Akhlaghi * lib/fitsarrayvv.c (pixelareaarcsec2): Previously called pixelsteradians. Changed the units to arcsec^2 because it is more useful. * bin/noisechisel/detection.c (detlabelsn): Now using a new sum of pixel values for flux weighted center of profile. The values are stored as one column in the 2015-07-07 Mohammad Akhlaghi * bin/mkcatalog/mkcatalog.c (firstpass): Use only positive (after subtracting sky) fluxes as weights for the flux weighted center. Also calculate the geometric center (irrespective of flux), so in case there are no positive pixels, the geometric center is output instead (after all, the object should be represented by some position and the NaN values that were used before are not useful). (secondpass): Similar to the above. Also I had simply replaced the getclumpinfo method of NoiseChisel's clumps.c here. But I had forgot that over there, all the neighboring clumps were within one detection. But here, two clumps could be one river pixel appart but belong to separate objects. So the wngb array has to have two values for each clump, not one, see the comments for more. Also I had to check the object IDs from the neighbors, not the river pixel. (setcpscorr): Removed. The minimum and maximum Standard deviations are now stored by NoiseChisel into the header of the standard deviation image. MakeProfiles then gets the value from those header parameters, so there was no need for this function. (makeoutput): The magnitude and S/N information is printed even if the user has not asked for magnitudes and S/Ns. * bin/mkcatalog/columns.c (sncol): Renamed variables to fit the clumpsntable function in bin/noisechisel/clumps.c. Also, the river flux is subtracted here, not before. * lib/fitsarrayvv.c: The numblank variable did not actually store the `number' of blank pixels, it was only a 0 or 1 value to specify if there are any blank pixels or not. It is now changed to `anyblank' to be more clear and not confuse the readers. All the Gnuastro programs that used this variable, were also corrected. 2015-07-06 Mohammad Akhlaghi * bin/noisechisel/noisechisel.c (noisechisel): After dilation, 4 connectivity was used to find the labels of the connected components. However, when we are looking around the river pixels in the segmentation process, we are looking in their 8-connected neighbors. So when two 4-connected labeled regions are separate, they can still be 8-connected and this will mess up the river flux association functions where the flux of a river is given to the clump that is touching it. It took me several frustrating hours to find this very simple bug! * bin/noisechisel/clumps.c (oversegment): NaN (masked) pixels are no longer fed into this function. So the conditions to check for them, especially in setting the top index are removed. (getclumpinfo): Now uses a different number for the sum of flux when trying to find the flux weighted center of the clump. This sum is made of only positive values. Negative values cannot act as weights and will mess up the center calculations. The new number for each column is stored in a third column to the xys array. Also, the xys array is no longer needed outside this function. 2015-07-05 Mohammad Akhlaghi * bin/mkcatalog/columns.c (brightnessfluxmag): Previously fluxmag. Now this function gives the brightness, flux and magnitude depending on its input parameters. * bin/mkcatalog/args.h (options): Corrected all usage of "flux" and "brightness". * doc/gnuastro.texi: Corrected all usage of "flux" and "brightness". * doc/forwebpage.sh (thismonth): Removed type=\"text/javascript\"" from the string since it seemed to be interfering with LibreJS. 2015-07-03 Mohammad Akhlaghi * lib/fitsarrayvv.c (readkeywords): Now reads multiple keywords. 2015-07-02 Mohammad Akhlaghi * bin/mkcatalog/mkcatalog.c (firstpass): Now accounts for blank labeled pixels. (setcpscorr): Now finds both the minimum and maximum of the STD, maximum for finding the 5sigma magnitude. * bin/mkcatalog/main.h (CATUNITMAG): Changed unit for magnitudes. 2015-06-26 Mohammad Akhlaghi * bin/noisechisel/thresh.c (qthreshonmesh): Only sort and find the quantile if there actually is any pixels! (applydetectionthresholdskysub): Now accounts for blank pixels. * bin/noisechisel/segmentation.c (segmentation): Now only works on non-blank pixels. * bin/noisechisel/label.c (BF_concmp): Now accounts for blank pixels in both unsigned char and long arrays. (labareas): Accounts for blank pixels. (removesmallarea_relabel): Accounts for blank pixels. (labindexs): Accounts for blank pixels. * bin/noisechisel/detection.c (detlabelsn): Now also removes detections in the sky area that cover a detection after filling holes. (removefalsedetections): Changed to applydetsn. (detsnthreshonmesh): Changed to detectpsedos. Practically this function just fills the holes in each large mesh and opens the binary result then puts the field back into the main p->dbyt array. It does not calculate anything any more. Such calculations have now become full image wide to find one S/N value over the full image. (detsnthreshongrid): Changed to detsnthresh. This function now does the image-wide calculations that were previously done by detsnthreshonmesh. (dbytolaboverlap): Now accounts for masked unsigned char and long arrays. * bin/noisechisel/clumps.c (clumpsntableonmesh): Previously clumpsnthreshonmesh. Moved all the countings and conditionals to another function to find the S/N threshold from one distribution over the image and not in the large meshs. (findclumpsn): Previously clumpsngrid. Now it collects all the S/N values from all the meshs into one array and uses that to find the S/N threshold using a fixed function for both detection and segmentation (snthresh in thresh.c). * bin/noisechisel/binary.c: The fixed value of 2 is changed BINARYNAN which is defined in binary.h. This makes managing the special values to use more easy, especially now that FITSBYTEBLANK is also being used from fitsarrayvv.h. (fh_makeinv): Replaced the old functions to fill the inverse array with new ones that don't use an index variable but pointers. It is much more cleaner, faster and easier to read now. It also now accounts for blank pixels and completely ignores them. (fillboundedholes): Similar to fh_makeinv. * bin/noisechisel/: The mesh based signal to noise calculations are now gone and one value is calculated for the full image. This allows for much better accuracy. Most of the steps in NoiseChisel were modified to take this into account. Also blank pixels are now included in the binary and labeled images too. * lib/fitsarrayvv.c (arraytofitsimg): Moved the BLANK keyword before EXTNAME. 2015-06-25 Mohammad Akhlaghi * bin/imgcrop/args.h (options): Changed inpolygon to outpolygon. Everywhere that inpolygon appeared, it is now outpolygon. * bin/imgcrop/wcsmode.c (wcscheckprepare): Check for both axises having the same pixel scale now incorporates floating point errors. * bin/imgcrop/crop.c (imgpolygonflpixel): Now gets the vertices and their number instead of the cropparams structure. This was done to make it be more general and use it in both Image mode and WCS mode. (onecrop): Allocation of the crp->ipolygon array was moved to the cropflpixel function. 2015-06-13 Mohammad Akhlaghi * lib/fitsarrayvv.c (fileorextname): New name for the setmaskname function. This was done to be a generic check, for all kinds of input, not just the mask. * bin/ : All the functions to make a copy of an input and print string values were changed. These were mainly in ui.c and args.h for each program. Until now, for each option, I would allocate, check and set the proper values, but now, I wrote a small function in checkset.c (allocatecopyset) which does the job. This makes reading the code significantly more easy and less bugy. 2015-06-12 Mohammad Akhlaghi * bin/subtractsky/args.h (options): Removed the --checkinterpolation option. * bin/subtractsky/subtractsky.c (subtractsky): Similar to below. * bin/noisechisel/thresh.c (findapplyqthreshold): Similar to below. * bin/noisechisel/sky.c (findavestdongrid): Similar to below. * bin/noisechisel/detection.c (findsnthreshongrid): Now using meshvaluefile from mesh.h instead of checking its self. Once the --meshbasedcheck was added, doing all the checks in each function was too long and repetative. So I just made this function to do the job with one call and not distract the readers. 2015-06-11 Mohammad Akhlaghi * bin/noisechisel/args.h (options): `minbfrac' and `minnumfalse' options moved under the `Input' category from the detections category. This move was because these two options are used by both the detection and segmentation steps and thus keeping them under detection would be confusing. Also `checkthresh' was changed to `checkthreshold'. Also, the option `numerosion' was changed to `erode' to be consistent with the opening and dilate options. 2015-06-10 Mohammad Akhlaghi * bin/mknoise/astmknoise.conf: Default background magnitude changed to -10 and zeropoint to 0.0. 2015-06-09 Mohammad Akhlaghi * bin/noisechisel/clumps.c: All functions now use the clumpsthreadparams structure as input instead of a list of arguments. (oversegment): ctp->topinds now keeps a good value when the clump has NaN pixels over it. * lib/mesh.c (imgindextomeshid): Corrected to work correctly when the pixel might be lying on the last mesh that might be larger. 2015-06-08 Mohammad Akhlaghi * bin/noisechisel/thresh.c (applydetectionthresholdskysub): Similar to below, uses p->imgss for sky subtracted image. * bin/noisechisel/sky.c (subtractskyimg): Does not touch the input image, puts the sky subtracted value in p->imgss. * bin/noisechisel/noisechisel.c (noisechisel): Removed the allocation of the mesh structures to ui.c * bin/noisechisel/detection.c (detlabelsn): Uses p->imgss for the sky subtracted image. 2015-06-07 Mohammad Akhlaghi * bin/mkprof/oneprofile.c (randompoints): The random number generator is now allocated (cloned) with the build thread and for every profile the seed is independently set once. Before each pixel would allocate and seed the random number generator individually! * bin/mkprof/astmkprof.conf: Changed default zeropoint magnitude to 0.00. * bin/mknoise/mknoise.c (mknoise): moved the random number generator to ui.c to make things faster and more easier to understand. * bin/mknoise/args.h (argp_option): Removed the `backgroundinmean' option, because I couldn't figure out what use it would have. If it is needed we can add it again later! * bin/imgstat/args.h (argp_option): Changed `binonzero' option to the more general `onebinvalue' option. * bin/convolve/convolve.c (removepaddingcorrectroundoff): Corrected bug: would return *d in both cases! It is corrected now. 2015-06-06 Mohammad Akhlaghi * lib/mesh.c (chbasedidfromgid): Chaged the old setmeshid to chbasedidfromgid along with a new function (gidfromchbasedid). The explanations on top of the first clearly explain everything extensively. The old function (my understanding) was not yet mature enough but now it seems to be very nicely working. All the functions that used this were also changed. * bin/noisechisel/astnoisechisel.conf: Changed default lastmeshfrac to 0.51 from 0.6. 2015-06-04 Mohammad Akhlaghi * bin/subtractsky/subtractsky.c (avestdonthread): No more need for setnan. Since all the meshes are initialized to NaN anyway. * lib/mesh.c: Previously, the garrays would be allocated and freed on every set of operations that were done on the mesh grid. I made some modifications so there is no more need to allocate and free them every time. A new prameter was added (ngarrays) so that on each use of the garrays, the number of garrays that are needed are kept here. All checks to work on the second garray are now done through this parameter. In this fashion, when multiple operations are to done on each mesh, there is no need to repeatedly free and allocate the garrays. Nearly all the functions in mesh.c were corrected to account for this. 2015-06-03 Mohammad Akhlaghi * bin/noisechisel/astnoisechisel.conf: Changed default dthresh to -0.1. * lib/statistics.c (histogram): Corrected the function. Until now, there was a problem when an element was on the last bin: it would go onto the next bin and thus would not be counted. This issue is now corrected. (cumulativefp): Same as above. 2015-06-02 Mohammad Akhlaghi * lib/mesh.c (operateonmesh): mp->indexs is now allocated in makemesh. Because all the programs that will need threads on meshs will need it, so it is best to set mp->indexs once and for all in makemesh. (meshinterponthread): Removed the naninds array, a new option was added to interpolate only on blank pixels when needed. (preparemeshinterparrays): Similar to the above. 2015-06-01 Mohammad Akhlaghi * lib/statistics.c: Removed all isnan checks in the comparison functions for the minimum and maximum values. NaN values will automatically fail all comparisons. * lib/timing.c (reporttiming): Removed the `in' from reporting seconds. * include/timing.h (VERBMSGLENGTH_V): Changed to 45 from 40. 2015-05-27 Mohammad Akhlaghi * bin/convolve/args.h (options): Remove the `noedgecorrection' option. Since it was useless. Also changed the old short option for spatial (`s') to `p'. Because `s' is now needed for the mesh size option. Also changed the old short option for khdu (`H') to `U', to make it similar to all the other programs that do convolution. * include/mesh.h (meshparams): the garrays are now only pointers. The allocated arrays are either cgarrays or fgarrays and based on the user's will, garray will be set equal to one of these two options. All the functions in mesh.c were changed to accomodate this change. 2015-05-25 Mohammad Akhlaghi * lib/mesh.c (operateonmesh): New name for `fillmesh'. Now the function that will be spinned off from each thread can be specified from the outside. 2015-05-24 Mohammad Akhlaghi * bin/imgcrop/crop.c (sectionparser): When only a `*' was given with no positive or negative following number, a segmentation fault would happen. This bug is now fixed. * lib/spatialconvolve.c (sconvonthread): No convolution will be attempted for a NaN pixel. 2015-05-23 Mohammad Akhlaghi * lib/mode.c (modesymmetricity): Corrrected topi to account for the case when 2*mi is larger than size. * bin/subtractsky/args.h: --numnearest and --kernelwidth moved to the `Mesh grid' part of the help output. --checksmoothing and --checkinterpolation also moved to the `Mesh grid' part. * lib/mesh.c (checkgarray): Modified to show both the full, or contiguous over full image, garray and the default one which is contiguous only over each channel. 2015-05-20 Mohammad Akhlaghi * lib/mode.c (modesymmetricity): Corrected topi to the end of the mirror distribution. (modesymmetricity): If no diff point is found, the end of the mirror distribution is used. Before it was the end of the data! (valuefromsym): af set to the quantile of the mirror distribution. 2015-05-18 Mohammad Akhlaghi * bin/convolve/convolve.c (complextoreal): Changed the two states to three to add only conerting the real part of an array. 2015-05-15 Mohammad Akhlaghi * bin/convolve/convolve.c (removepaddingcorrectroundoff): The limit to check for floating point errors is now set by a macro and changed to 1e-10 instead of 1e-17. * lib/statistics.c (sigmaclip_converge): Now, there is a limit on the number of times to try for convergence. * lib/mode.c (makemirrorplots): All the output paramters are now given as arguments so the output can be fully configured from the outside. Also, the method that it sets the plot ranges is now better configurable. * include/mode.h (MODESYMGOOD): Changed to 0.2 from 0.15 based on new simulation tests. 2015-05-11 Mohammad Akhlaghi * lib/statistics.c (setbins): Changed method to find the bin that has the value zero within it. Before it would just choose the first bin with a positive value. But now, it will check the signs of the two interval sides of the bin and when ever the multiplication becomes negative, that bin is chosen. (histogram): Changed so the last bin is a closed bin, not half open like the rest of the histogram bins. This also includes floating point rounding error. (cumulativefp): Same as the histogram function. (sigmaclip_certainnum): Printing is now an option. (sigmaclip_converge): Printing is now an option. * lib/mode.c (makemirrorplots): New name for the old savemodeplots. * include/mode.h: Changed input arguments to modeindexinsorted. Plots can now be made through the separate makemirrorpolots function. 2015-05-05 Mohammad Akhlaghi * bin/subtractsky/ui.c (preparearrays): Moved the function that reads any input as float and incorporates the mask into it. * include/fixedstringmacros.h (MOREHELPINFO): Removed long explanation about help-gnuastro. Instead an info link to the part of the manual that introduces it was included. 2015-05-03 Mohammad Akhlaghi * include/fixedstringmacros.h (MOREHELPINFO): Corrected to include help-gnuastro mailing list. * doc/style.css (a:hover): Changed to bright orange color. (a:active): Changed to dark orange. 2015-04-24 Mohammad Akhlaghi * bin/mkprof/oneprofile.c (makepixbypix): When in circumference mode, if the truncation radius is reached, it is filled with the profile value. This is done so very elongated profiles can at least show a one pixel circumference. * bin/mkprof/main.h (MINCIRCUMWIDTH): Changed to 0.5f. * lib/checkset.c (doublelvalue): Corrected bad value report when options are called. 2015-04-21 Mohammad Akhlaghi * bin/mkprof/ui.c (freeandreport): Avoided double-free by only freeing mergeedimgname when it is not equal to output. * bin/mkprof/oneprofile.c (makepixbypix): Will only do monte carlo integration when the profile is not a constant value. (setprofparams): Changed the function of point to `Fixed'. * bin/mkprof/mkprof.c (write): Changed to replace and read from an image and add profiles on that. * lib/statistics.c: All float and double functions can now work with NaN too. * bin/mkprof/ui.c (setparams): Catalog is always given, no need to check. * doc/gnuastro.texi: Removed all "Future updates ..." subsections in the manual. They are now managed in the Gnuastro project webpage on Savannah. 2015-04-13 Mohammad Akhlaghi * lib/fitsarrayvv.c (updatekeys): When no value is given, it will use fits_update_key_null. (readwcs): Uses fits_free_memory instead of clib's free. 2015-04-06 Mohammad Akhlaghi * bin/mkprof/mkprof.c: Corrected condition when a thread would finish `build' profiles but the last set of its profiles wouldn't pass onto `write'. * bin/mknoise/: Changed background flux unit to magnitudes, not flux. * THANKS: Added institutions which also helped. 2015-04-03 Mohammad Akhlaghi * lib/fitsarrayvv.c: Changed all occurences of `nul' or `NUL' to `blank' or `BLANK'. The FITS standard defines a BLANK keyword for integer types. (copyrightandend): Will now right extra headers. (arraytofitsimg): Can now accept header to write to output. * include/fitsarrayvv.h: Changed all `NUL' macros to `BLANK'. 2015-04-02 Mohammad Akhlaghi * lib/fitsarrayvv.c (changetype): Round floating point input types for integer output types. (arraytofitsimg): Added numblank as a variable, to deal with blank pixels. * bin/imgwarp/imgwarp.c (imgwarppreparations): Coorected the point (1.0f, 1.0f) to be center of the first pixel, not zero. * lib/fitsarrayvv.c (copyrightandend): Removed the Copyright notice of Gnuastro from the output image header. Since it might be confused with a copyright on the data its self. 2015-04-01 Mohammad Akhlaghi * bin/imgwarp/args.h: Temporarily removed the wrap option. Will be added later. 2015-03-24 Mohammad Akhlaghi * bin/imgcrop/ui.c (preparearrays): Aborts if in WCS mode and the wcsprm structure could not be started. * bin/imgcrop/crop.c (firstcropmakearray): Only adds WCS headers if the wcsprm structure is defined. * lib/fitsarrayvv.c (readwcs): If any error occurs, a warning message will be printed and the returned pointer will be NULL. 2015-03-17 Mohammad Akhlaghi * tests/convertt/: If libjpeg is not present, the tests will be skipped. * bin/convertt/: libjpeg is now optional. * configure.ac: Changed libjpeg to an optional requirement. So if it is not available, Gnuastro can still be built. 2015-03-16 Mohammad Akhlaghi * bin/convolve/ui.c (preparearrays): The flip parts was missing a -1. * doc/gnuastro.texi: Changed all `gnuastro' occurrences in the text to `Gnuastro'. 2015-03-14 Mohammad Akhlaghi * bin/convolve/convolve.c: Added frequency domain convolution. 2015-03-12 Mohammad Akhlaghi * bin/mkprof/ui.c (setparams): Added condition for no output given. * bin/mkprof/astmkprof.conf: Removed output. * bin/imgcrop/ui.c (sanitycheck): Moved check of reentrancy in cfitsio to the end so if numthreads is set to 1, there is no problem. * bin/convertt/ui.c (sanitycheck): Added check if output is not set. * bin/convertt/astconvertt.conf: Removed output. * lib/spatialconvolve.c: First version complete. * configure.ac: Removed sqrt and pthread tests (they are done by Gnulib). Added the AX_PTHREAD macro from Autoconf archives. 2015-03-11 Mohammad Akhlaghi * bin/convolve/: Adding new functions and steps. * ./: Copyright transferred to the FSF. Copyright notices in all files changed. 2015-03-10 Mohammad Akhlaghi * tests/imgcrop/*.sh: Set --numthreads=1 for all the tests so if CFITSIO is not installed with reentrancy, there is no failures. * tests/Makefile.am: Made the fitstopdf result conditional on if GPL GhostScript is installed. * include/astrthreads.c: Removed the old function and structure for replacing the pthread_barrier type and functions that was copy and pasted from another webpage and replaced it with my own implementation. * configure.ac: bug report email set. pthread_barrier checked. GPL GhostScript checked. 2015-03-09 Mohammad Akhlaghi * include/astrthreads.h: Added a temporary function so the pthread_barrier type and functions can be run on systems that don't support it. I have contacted the author and it will only remain if he clarifies the license. I have also asked the Gnulib people to try to include it so this issue can be completely fixed. * configure.ac: Added checks for nproc and gs along with warnings. 2015-03-02 Mohammad Akhlaghi * bin/convolve/: Work started on Convolve. * lib/fitsarrayvv.c: Changed array types from intXX_t to short, long and LONGLONG. Unfortuantely this is how CFITSIO works. 2015-02-22 Mohammad Akhlaghi * doc/gnuastro.texi: Added index, changed "Science and its software". 2015-02-20 Mohammad Akhlaghi * doc/gnuastro.texi: Removed list of programs at first, added a programs index. Added an examples chapter along with some one line examples of each program. Moved the Why C and design philosophy subsections to the Developing chapters. * src: All 'error' functions are now called with a string literal and not a string variable. Also all 'system' function calls now check the return value. * lib: Similar to above. * include: similar to above. 2015-02-18 Mohammad Akhlaghi * lib/Makefile.am: Changed all static libraries to libtool static libraries. * doc/gnuastro.texi: Updated. * configure.ac: Added Libtool checks. Corrected cfitsio and wcslib dependencies and removed FFTW as a dependency. 2015-02-17 Mohammad Akhlaghi * bin/convertt/eps.c: Functions for binary image added. * lib/fitsarrayvv.c (nameisfits): Check length. * doc/gnuastro.texi (Internal libraries): Removed details of libraries. * README: Details removed. 2015-02-16 Mohammad Akhlaghi * lib/statistics.c (dminmax): Works with NAN values too. (fminmax): Similar to dminmax. * doc/gnuastro.texi (ConvertType): Updated. 2015-02-13 Mohammad Akhlaghi * bin/convertt/args.h (argp_options): `convert` changed to `change`. Since the program name is also convert this could cause confusions. * doc/gnuastro.texi (Invoking astconvertt): Option explanations. * bin/convertt/jpeg.c (savejpeg): Corrected the pixel ordering. * bin/convertt/convertt.c (doubleto8bit): Find minimum and maximum for all colors to set the scale, not just one color. * lib/fitsarrayvv.c (arraytofitsimg): Will not remove comments. * include/fixedstringmacros.h (SHORTCOPYRIGHT): Corrected year. * lib/fitsarrayvv.c (nameisfits): Dot no longer included. (nameisfitssuffix): Added. (changetype): Corrected input and output pointers. * doc/gnuastro.texi (ConvertType): Added explanations. (Future updates): Chapter removed. 2015-02-11 Mohammad Akhlaghi * bin/convertt/ui.c (preparearrays): Added. * bin/convertt/jpeg.c (preparejpeg): Added. * doc/gnuastro.texi (Files): Added chapter (ConvertType): Added section (FileInfo): Added section 2015-02-08 Mohammad Akhlaghi * bin/convertt: Started working on ConvertType. * lib/checkset.c (intsmallerequalto): Function Added. * include/fixedstringmacros.h (ASTRUTILSBIBTEX): Corrected article name * include/checkset.h: Added intsmallerequalto. 2015-01-25 Mohammad Akhlaghi * ./*: In all files, the name `AstrUtils` was changed to `gnuastro` and the `astr` prefix was changed to `ast`. 2015-01-20 Mohammad Akhlaghi * tests/imgcrop/makerandomcat.py: Removed, because now the points are very specific. * tests/imgcrop/*.sh: Corrected the inputs to the outputs of MakeProfiles tests. * tests/Makefile.am (TESTS): Added tests for MakeProfiles. * Makefile.am (EXTRA_DIST): Moved the distribution files for each folder to the Makefile.am in that folder. 2015-01-19 Mohammad Akhlaghi * bin/mkprof/ui.c: Steps for reading and checking WCS parameters added. * bin/mkprof/oneprofile.c (ispsf): Added for a fixed place to check if a profile is a PSF. (makeoneprofile): Finding mkp->xc and mkp->yc moved here. * bin/mkprof/mkprof.c (preparewcs): Added. (build): Removed finding mkp->xc and mkp->yc. * bin/mkprof/args.h (argp_option): Added WCS related options. * bin/imgcrop/imgcrop.c (imgcrop): Number of barriers, corrected for when the number of jobs was less than the number of threads. * lib/fitsarrayvv.c (addwcstoheader): Changed the WCS structure to the WCS header string as input. (arraytofitsimg): Convert the WCS structure and remove the comments CFITSIO in here. (atofcorrectwcs): Added. * doc/astrutils.texi: Updated. 2015-01-18 Mohammad Akhlaghi * bin/mkprof/mkprof.c (writelog): Added. (write): Completed. * bin/mkprof/args.h (arg_option): Added `--nomerged`. * lib/txtarrayvv.c (doformatting): Added option to use `f` in printf or `g`. 2015-01-16 Mohammad Akhlaghi * bin/mkprof/mkprof.c (builtqueue_addempty): Added. (saveindividual): Added. (build): Is working until the profile is built. * bin/mkprof/ellipse.h: Function taken to `box.h`. * bin/mkprof/ellipse.c: Function taken to `box.c`. * bin/mkprof/args.h (argp_option): added `--numrandom`, changed `mginimg` to `psfinimg`. * bin/imgcrop/main.h (imgcropparams): iwidth is now a 2 element array. * bin/imgcrop/crop.c: Removed `borderfromcenter` and `correctflpixels` to `lib/box.c`. * lib/stats.h: Changed to `statistics.h`, all non-used functions removed. * lib/arraymanip.c: Removed all non-used functions. * include/stats.h: Changed to `statistics.h` and all non-used functions removed. * include/fixedstringmacros.h (ASTRUTILSBIBTEX): Added. * include/commonargs.h (argp_option): Added `--cite` option and added the `main.h` and `cite.h` header for each program to use their names. * include/checkset.h: function name `nameiswritable` is changed to dir0file1 which is much more descriptive. * include/arraymanip.h: Removed all the non-used functions from the past. New functions will be added as they are needed. * doc/astrutils.texi: Updated. 2015-01-13 Mohammad Akhlaghi * bin/mkprof/ui.c (preparearrays): Added. (setparams): numthreads initialized to configured value. * bin/mkprof/mkprof.c (build): Added. (write): Added. (mkprof): Parallel jobs configured. * bin/mkprof/ellipse.c: Added * bin/mkprof/args.h (argp_option): Changed psfprofsinimg to mginimg. * bin/imgcrop/imgcrop.c (imgcrop): Used attrbarrierinit. * lib/astrthreads.c (attrbarrierinit): Added. * doc/astrutils.texi: Updated. 2015-01-12 Mohammad Akhlaghi * bin/imgcrop/imgcrop.c: Using pthread_barrier_wait for synchronizing threads instead of the mutexes and conditional variables before. * lib/txtarrayvv.c: When the value couldn't be read as a number, it would be saved as the lowest possible double value. Now it will be saved as a NaN. * lib/fitsarrayvv.c (nultovalue): Convert blank values in images to a given values. (changetype): Change the type of an image. * lib/checkset.c (nameisawritablefile): Corrected to accurately check if the given name is usable as output. * lib/arraymanip.c (converttofloat): Removed conversion functions. These were mainly for converting a FITS image type to the desired type. Now there is one function in fitsarrayvv.c which will do the conversion. * include/checkset.h (CHECKCOLINCAT): Added to check column number and all values within a column. * doc/astrutils.texi: Updated the text, changing names and explanations. * configure.ac: Changed MockGals, mockgals, name to MakeProfiles, mkprof. * Makefile.am (EXTRA_DIST): Moved the library header files to the Makefile.am in lib/. 2015-01-06 Mohammad Akhlaghi * bin/mockgals/args.h (parse_opt): Removed the check below. * bin/imgcrop/args.h (parse_opt): Removed the check below. * include/commonargs.h (cparse_opt): Added check for not calling `--setdirconf` and `--setusrconf` together. 2015-01-05 Mohammad Akhlaghi * doc/formath.texi: Added. A set of macros to write equations nicely in TeX, HTML (using MathJax). * bin/imgcrop/astrimgcrop.def: renamed to bin/imgcrop/astrimgcrop.conf. * lib/defaults.c: renamed to include/configfiles.c. * lib/checkset.c (stringhasspace): Function added. * include/fixedstringmacros.h (SHORTCOPYRIGHT): 2015 added. (MOREHELPINFO): Corrected info explanation in help output. * include/defaults.h: renamed to include/configfiles.h * include/commonparams.h (commonparams): Similar to the change in commonargs.h. * include/commonargs.h (argp_option): `--dirdefaults` and `--userdefaults` changed to `--setdirconf` and `--setusrconf`. * doc/astrutils.texi: Included formath.texi to display math equations, updates to the text. * doc/Makefile.am (headers): Used a shell '*' instead of calling each program separately. This was enabled with the new file structure. * configure.ac: Changed all default names to configure for a configuration file, not a default file (only name). * Makefile.am: MockGals conditional compilation added. 2014-12-30 Mohammad Akhlaghi * tests/basicchecks.sh: New file (common tests for all tests). * tests/Makefile.am (AM_TESTS_ENVIRONMENT): Corrected test environment. * bin/imgcrop/ui.c (setparams): Moved all similar actions to the CHECKSETDEFAULTS macro in defaults.h * bin/imgcrop/Makefile.am (AM_CPPFLAGS): New (previously in AM_CFLAGS). * lib/defaults.c (addhomedir): Now returns char *. (writelocaldefaultstop): Informs the user of how to make the needed directory with `make -p`. * include/defaults.h (SAVE_LOCAL_DEFAULTS): changed addhomedir. (CHECKSETDEFAULTS): A new macro to read defaults. (END_OF_NOTSET_REPORT): Added some extra information. * doc/astrutils.texi: A lot of updates in the text! Listing them all would be too much! * configure.ac: `--with-numthreads` and `--enable-progname` were created along with all their necessary checks. * Makefile.am: Set conditional subdirectories. Added `basicchecks.sh` to the files to be distributed. 2014-12-28 Mohammad Akhlaghi GNU Astronomical Utilities created with the ImageCrop as the first package. Other packages will be added in the next few days. gnuastro-0.2.33-8a3b/COPYING0000644000175000017500000010451312720642724012162 00000000000000 GNU GENERAL PUBLIC LICENSE Version 3, 29 June 2007 Copyright (C) 2007 Free Software Foundation, Inc. Everyone is permitted to copy and distribute verbatim copies of this license document, but changing it is not allowed. Preamble The GNU General Public License is a free, copyleft license for software and other kinds of works. The licenses for most software and other practical works are designed to take away your freedom to share and change the works. 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Notwithstanding any other provision of this License, for material you add to a covered work, you may (if authorized by the copyright holders of that material) supplement the terms of this License with terms: a) Disclaiming warranty or limiting liability differently from the terms of sections 15 and 16 of this License; or b) Requiring preservation of specified reasonable legal notices or author attributions in that material or in the Appropriate Legal Notices displayed by works containing it; or c) Prohibiting misrepresentation of the origin of that material, or requiring that modified versions of such material be marked in reasonable ways as different from the original version; or d) Limiting the use for publicity purposes of names of licensors or authors of the material; or e) Declining to grant rights under trademark law for use of some trade names, trademarks, or service marks; or f) Requiring indemnification of licensors and authors of that material by anyone who conveys the material (or modified versions of it) with contractual assumptions of liability to the recipient, for any liability that these contractual assumptions directly impose on those licensors and authors. All other non-permissive additional terms are considered "further restrictions" within the meaning of section 10. If the Program as you received it, or any part of it, contains a notice stating that it is governed by this License along with a term that is a further restriction, you may remove that term. If a license document contains a further restriction but permits relicensing or conveying under this License, you may add to a covered work material governed by the terms of that license document, provided that the further restriction does not survive such relicensing or conveying. If you add terms to a covered work in accord with this section, you must place, in the relevant source files, a statement of the additional terms that apply to those files, or a notice indicating where to find the applicable terms. Additional terms, permissive or non-permissive, may be stated in the form of a separately written license, or stated as exceptions; the above requirements apply either way. 8. Termination. You may not propagate or modify a covered work except as expressly provided under this License. Any attempt otherwise to propagate or modify it is void, and will automatically terminate your rights under this License (including any patent licenses granted under the third paragraph of section 11). However, if you cease all violation of this License, then your license from a particular copyright holder is reinstated (a) provisionally, unless and until the copyright holder explicitly and finally terminates your license, and (b) permanently, if the copyright holder fails to notify you of the violation by some reasonable means prior to 60 days after the cessation. Moreover, your license from a particular copyright holder is reinstated permanently if the copyright holder notifies you of the violation by some reasonable means, this is the first time you have received notice of violation of this License (for any work) from that copyright holder, and you cure the violation prior to 30 days after your receipt of the notice. Termination of your rights under this section does not terminate the licenses of parties who have received copies or rights from you under this License. If your rights have been terminated and not permanently reinstated, you do not qualify to receive new licenses for the same material under section 10. 9. Acceptance Not Required for Having Copies. You are not required to accept this License in order to receive or run a copy of the Program. Ancillary propagation of a covered work occurring solely as a consequence of using peer-to-peer transmission to receive a copy likewise does not require acceptance. However, nothing other than this License grants you permission to propagate or modify any covered work. These actions infringe copyright if you do not accept this License. Therefore, by modifying or propagating a covered work, you indicate your acceptance of this License to do so. 10. Automatic Licensing of Downstream Recipients. Each time you convey a covered work, the recipient automatically receives a license from the original licensors, to run, modify and propagate that work, subject to this License. You are not responsible for enforcing compliance by third parties with this License. An "entity transaction" is a transaction transferring control of an organization, or substantially all assets of one, or subdividing an organization, or merging organizations. If propagation of a covered work results from an entity transaction, each party to that transaction who receives a copy of the work also receives whatever licenses to the work the party's predecessor in interest had or could give under the previous paragraph, plus a right to possession of the Corresponding Source of the work from the predecessor in interest, if the predecessor has it or can get it with reasonable efforts. You may not impose any further restrictions on the exercise of the rights granted or affirmed under this License. For example, you may not impose a license fee, royalty, or other charge for exercise of rights granted under this License, and you may not initiate litigation (including a cross-claim or counterclaim in a lawsuit) alleging that any patent claim is infringed by making, using, selling, offering for sale, or importing the Program or any portion of it. 11. Patents. A "contributor" is a copyright holder who authorizes use under this License of the Program or a work on which the Program is based. The work thus licensed is called the contributor's "contributor version". A contributor's "essential patent claims" are all patent claims owned or controlled by the contributor, whether already acquired or hereafter acquired, that would be infringed by some manner, permitted by this License, of making, using, or selling its contributor version, but do not include claims that would be infringed only as a consequence of further modification of the contributor version. For purposes of this definition, "control" includes the right to grant patent sublicenses in a manner consistent with the requirements of this License. Each contributor grants you a non-exclusive, worldwide, royalty-free patent license under the contributor's essential patent claims, to make, use, sell, offer for sale, import and otherwise run, modify and propagate the contents of its contributor version. In the following three paragraphs, a "patent license" is any express agreement or commitment, however denominated, not to enforce a patent (such as an express permission to practice a patent or covenant not to sue for patent infringement). To "grant" such a patent license to a party means to make such an agreement or commitment not to enforce a patent against the party. If you convey a covered work, knowingly relying on a patent license, and the Corresponding Source of the work is not available for anyone to copy, free of charge and under the terms of this License, through a publicly available network server or other readily accessible means, then you must either (1) cause the Corresponding Source to be so available, or (2) arrange to deprive yourself of the benefit of the patent license for this particular work, or (3) arrange, in a manner consistent with the requirements of this License, to extend the patent license to downstream recipients. "Knowingly relying" means you have actual knowledge that, but for the patent license, your conveying the covered work in a country, or your recipient's use of the covered work in a country, would infringe one or more identifiable patents in that country that you have reason to believe are valid. If, pursuant to or in connection with a single transaction or arrangement, you convey, or propagate by procuring conveyance of, a covered work, and grant a patent license to some of the parties receiving the covered work authorizing them to use, propagate, modify or convey a specific copy of the covered work, then the patent license you grant is automatically extended to all recipients of the covered work and works based on it. A patent license is "discriminatory" if it does not include within the scope of its coverage, prohibits the exercise of, or is conditioned on the non-exercise of one or more of the rights that are specifically granted under this License. You may not convey a covered work if you are a party to an arrangement with a third party that is in the business of distributing software, under which you make payment to the third party based on the extent of your activity of conveying the work, and under which the third party grants, to any of the parties who would receive the covered work from you, a discriminatory patent license (a) in connection with copies of the covered work conveyed by you (or copies made from those copies), or (b) primarily for and in connection with specific products or compilations that contain the covered work, unless you entered into that arrangement, or that patent license was granted, prior to 28 March 2007. Nothing in this License shall be construed as excluding or limiting any implied license or other defenses to infringement that may otherwise be available to you under applicable patent law. 12. No Surrender of Others' Freedom. If conditions are imposed on you (whether by court order, agreement or otherwise) that contradict the conditions of this License, they do not excuse you from the conditions of this License. If you cannot convey a covered work so as to satisfy simultaneously your obligations under this License and any other pertinent obligations, then as a consequence you may not convey it at all. For example, if you agree to terms that obligate you to collect a royalty for further conveying from those to whom you convey the Program, the only way you could satisfy both those terms and this License would be to refrain entirely from conveying the Program. 13. Use with the GNU Affero General Public License. Notwithstanding any other provision of this License, you have permission to link or combine any covered work with a work licensed under version 3 of the GNU Affero General Public License into a single combined work, and to convey the resulting work. The terms of this License will continue to apply to the part which is the covered work, but the special requirements of the GNU Affero General Public License, section 13, concerning interaction through a network will apply to the combination as such. 14. Revised Versions of this License. The Free Software Foundation may publish revised and/or new versions of the GNU General Public License from time to time. Such new versions will be similar in spirit to the present version, but may differ in detail to address new problems or concerns. Each version is given a distinguishing version number. If the Program specifies that a certain numbered version of the GNU General Public License "or any later version" applies to it, you have the option of following the terms and conditions either of that numbered version or of any later version published by the Free Software Foundation. If the Program does not specify a version number of the GNU General Public License, you may choose any version ever published by the Free Software Foundation. If the Program specifies that a proxy can decide which future versions of the GNU General Public License can be used, that proxy's public statement of acceptance of a version permanently authorizes you to choose that version for the Program. Later license versions may give you additional or different permissions. However, no additional obligations are imposed on any author or copyright holder as a result of your choosing to follow a later version. 15. Disclaimer of Warranty. THERE IS NO WARRANTY FOR THE PROGRAM, TO THE EXTENT PERMITTED BY APPLICABLE LAW. EXCEPT WHEN OTHERWISE STATED IN WRITING THE COPYRIGHT HOLDERS AND/OR OTHER PARTIES PROVIDE THE PROGRAM "AS IS" WITHOUT WARRANTY OF ANY KIND, EITHER EXPRESSED OR IMPLIED, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE. THE ENTIRE RISK AS TO THE QUALITY AND PERFORMANCE OF THE PROGRAM IS WITH YOU. SHOULD THE PROGRAM PROVE DEFECTIVE, YOU ASSUME THE COST OF ALL NECESSARY SERVICING, REPAIR OR CORRECTION. 16. Limitation of Liability. IN NO EVENT UNLESS REQUIRED BY APPLICABLE LAW OR AGREED TO IN WRITING WILL ANY COPYRIGHT HOLDER, OR ANY OTHER PARTY WHO MODIFIES AND/OR CONVEYS THE PROGRAM AS PERMITTED ABOVE, BE LIABLE TO YOU FOR DAMAGES, INCLUDING ANY GENERAL, SPECIAL, INCIDENTAL OR CONSEQUENTIAL DAMAGES ARISING OUT OF THE USE OR INABILITY TO USE THE PROGRAM (INCLUDING BUT NOT LIMITED TO LOSS OF DATA OR DATA BEING RENDERED INACCURATE OR LOSSES SUSTAINED BY YOU OR THIRD PARTIES OR A FAILURE OF THE PROGRAM TO OPERATE WITH ANY OTHER PROGRAMS), EVEN IF SUCH HOLDER OR OTHER PARTY HAS BEEN ADVISED OF THE POSSIBILITY OF SUCH DAMAGES. 17. Interpretation of Sections 15 and 16. If the disclaimer of warranty and limitation of liability provided above cannot be given local legal effect according to their terms, reviewing courts shall apply local law that most closely approximates an absolute waiver of all civil liability in connection with the Program, unless a warranty or assumption of liability accompanies a copy of the Program in return for a fee. END OF TERMS AND CONDITIONS How to Apply These Terms to Your New Programs If you develop a new program, and you want it to be of the greatest possible use to the public, the best way to achieve this is to make it free software which everyone can redistribute and change under these terms. To do so, attach the following notices to the program. It is safest to attach them to the start of each source file to most effectively state the exclusion of warranty; and each file should have at least the "copyright" line and a pointer to where the full notice is found. Copyright (C) This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . Also add information on how to contact you by electronic and paper mail. If the program does terminal interaction, make it output a short notice like this when it starts in an interactive mode: Copyright (C) This program comes with ABSOLUTELY NO WARRANTY; for details type `show w'. This is free software, and you are welcome to redistribute it under certain conditions; type `show c' for details. The hypothetical commands `show w' and `show c' should show the appropriate parts of the General Public License. Of course, your program's commands might be different; for a GUI interface, you would use an "about box". You should also get your employer (if you work as a programmer) or school, if any, to sign a "copyright disclaimer" for the program, if necessary. For more information on this, and how to apply and follow the GNU GPL, see . The GNU General Public License does not permit incorporating your program into proprietary programs. If your program is a subroutine library, you may consider it more useful to permit linking proprietary applications with the library. If this is what you want to do, use the GNU Lesser General Public License instead of this License. But first, please read . gnuastro-0.2.33-8a3b/AUTHORS0000644000175000017500000000046613004464663012201 00000000000000GNU Astronomy Utilities (Gnuastro) authors ========================================== Generated for Gnuastro 0.2.33-8a3b. Ordered by number of commits in the Git project history. 487 Mohammad Akhlaghi 29 Mosè Giordano 12 Vladimir Markelov gnuastro-0.2.33-8a3b/config.h.in0000644000175000017500000020153513004464626013153 00000000000000/* config.h.in. Generated from configure.ac by autoheader. */ /* Define if building universal (internal helper macro) */ #undef AC_APPLE_UNIVERSAL_BUILD /* Define to the number of bits in type 'ptrdiff_t'. */ #undef BITSIZEOF_PTRDIFF_T /* Define to the number of bits in type 'sig_atomic_t'. */ #undef BITSIZEOF_SIG_ATOMIC_T /* Define to the number of bits in type 'size_t'. */ #undef BITSIZEOF_SIZE_T /* Define to the number of bits in type 'wchar_t'. */ #undef BITSIZEOF_WCHAR_T /* Define to the number of bits in type 'wint_t'. */ #undef BITSIZEOF_WINT_T /* Date of compilation */ #undef CONFIGDATE /* Time of compilation */ #undef CONFIGTIME /* Configuration file post fix. */ #undef CONF_POSTFIX /* Configuration file name format. */ #undef CONF_SHOWFMT /* Define to one of `_getb67', `GETB67', `getb67' for Cray-2 and Cray-YMP systems. This function is required for `alloca.c' support on those systems. */ #undef CRAY_STACKSEG_END /* Local data dir. */ #undef CURDIRCONFIG_DIR /* Define to 1 if using `alloca.c'. */ #undef C_ALLOCA /* Define to 1 if the C locale may have encoding errors. */ #undef C_LOCALE_MAYBE_EILSEQ /* Define as the bit index in the word where to find bit 0 of the exponent of 'double'. */ #undef DBL_EXPBIT0_BIT /* Define as the word index where to find the exponent of 'double'. */ #undef DBL_EXPBIT0_WORD /* Define to 1 if // is a file system root distinct from /. */ #undef DOUBLE_SLASH_IS_DISTINCT_ROOT /* Define to nothing if C supports flexible array members, and to 1 if it does not. That way, with a declaration like 'struct s { int n; double d[FLEXIBLE_ARRAY_MEMBER]; };', the struct hack can be used with pre-C99 compilers. When computing the size of such an object, don't use 'sizeof (struct s)' as it overestimates the size. Use 'offsetof (struct s, d)' instead. Don't use 'offsetof (struct s, d[0])', as this doesn't work with MSVC and with C++ compilers. */ #undef FLEXIBLE_ARRAY_MEMBER /* Define to 1 if nl_langinfo (YESEXPR) returns a non-empty string. */ #undef FUNC_NL_LANGINFO_YESEXPR_WORKS /* libgit2 is installed on the system */ #undef GAL_GNUASTRO_HAVE_LIBGIT2 /* System has pthread_barrier */ #undef GAL_GNUASTRO_HAVE_PTHREAD_BARRIER /* Define if gettimeofday clobbers the localtime buffer. */ #undef GETTIMEOFDAY_CLOBBERS_LOCALTIME /* Define this to 'void' or 'struct timezone' to match the system's declaration of the second argument to gettimeofday. */ #undef GETTIMEOFDAY_TIMEZONE /* Define to a C preprocessor expression that evaluates to 1 or 0, depending whether the gnulib module fscanf shall be considered present. */ #undef GNULIB_FSCANF /* Define to a C preprocessor expression that evaluates to 1 or 0, depending whether the gnulib module lock shall be considered present. */ #undef GNULIB_LOCK /* Define to a C preprocessor expression that evaluates to 1 or 0, depending whether the gnulib module malloc-gnu shall be considered present. */ #undef GNULIB_MALLOC_GNU /* Define to 1 if printf and friends should be labeled with attribute "__gnu_printf__" instead of "__printf__" */ #undef GNULIB_PRINTF_ATTRIBUTE_FLAVOR_GNU /* Define to 1 to add extern declaration of program_invocation_name to argp.h */ #undef GNULIB_PROGRAM_INVOCATION_NAME /* Define to 1 to add extern declaration of program_invocation_short_name to argp.h */ #undef GNULIB_PROGRAM_INVOCATION_SHORT_NAME /* Define to a C preprocessor expression that evaluates to 1 or 0, depending whether the gnulib module scanf shall be considered present. */ #undef GNULIB_SCANF /* Define to a C preprocessor expression that evaluates to 1 or 0, depending whether the gnulib module strerror shall be considered present. */ #undef GNULIB_STRERROR /* Define to 1 when the gnulib module btowc should be tested. */ #undef GNULIB_TEST_BTOWC /* Define to 1 when the gnulib module close should be tested. */ #undef GNULIB_TEST_CLOSE /* Define to 1 when the gnulib module dup2 should be tested. */ #undef GNULIB_TEST_DUP2 /* Define to 1 when the gnulib module environ should be tested. */ #undef GNULIB_TEST_ENVIRON /* Define to 1 when the gnulib module fdopen should be tested. */ #undef GNULIB_TEST_FDOPEN /* Define to 1 when the gnulib module fstat should be tested. */ #undef GNULIB_TEST_FSTAT /* Define to 1 when the gnulib module getcwd should be tested. */ #undef GNULIB_TEST_GETCWD /* Define to 1 when the gnulib module getdtablesize should be tested. */ #undef GNULIB_TEST_GETDTABLESIZE /* Define to 1 when the gnulib module getopt-gnu should be tested. */ #undef GNULIB_TEST_GETOPT_GNU /* Define to 1 when the gnulib module getpagesize should be tested. */ #undef GNULIB_TEST_GETPAGESIZE /* Define to 1 when the gnulib module gettimeofday should be tested. */ #undef GNULIB_TEST_GETTIMEOFDAY /* Define to 1 when the gnulib module localeconv should be tested. */ #undef GNULIB_TEST_LOCALECONV /* Define to 1 when the gnulib module lstat should be tested. */ #undef GNULIB_TEST_LSTAT /* Define to 1 when the gnulib module malloc-posix should be tested. */ #undef GNULIB_TEST_MALLOC_POSIX /* Define to 1 when the gnulib module mbrtowc should be tested. */ #undef GNULIB_TEST_MBRTOWC /* Define to 1 when the gnulib module mbsinit should be tested. */ #undef GNULIB_TEST_MBSINIT /* Define to 1 when the gnulib module mbtowc should be tested. */ #undef GNULIB_TEST_MBTOWC /* Define to 1 when the gnulib module memchr should be tested. */ #undef GNULIB_TEST_MEMCHR /* Define to 1 when the gnulib module mempcpy should be tested. */ #undef GNULIB_TEST_MEMPCPY /* Define to 1 when the gnulib module nl_langinfo should be tested. */ #undef GNULIB_TEST_NL_LANGINFO /* Define to 1 when the gnulib module open should be tested. */ #undef GNULIB_TEST_OPEN /* Define to 1 when the gnulib module putenv should be tested. */ #undef GNULIB_TEST_PUTENV /* Define to 1 when the gnulib module rawmemchr should be tested. */ #undef GNULIB_TEST_RAWMEMCHR /* Define to 1 when the gnulib module setenv should be tested. */ #undef GNULIB_TEST_SETENV /* Define to 1 when the gnulib module setlocale should be tested. */ #undef GNULIB_TEST_SETLOCALE /* Define to 1 when the gnulib module sleep should be tested. */ #undef GNULIB_TEST_SLEEP /* Define to 1 when the gnulib module stat should be tested. */ #undef GNULIB_TEST_STAT /* Define to 1 when the gnulib module strchrnul should be tested. */ #undef GNULIB_TEST_STRCHRNUL /* Define to 1 when the gnulib module strerror should be tested. */ #undef GNULIB_TEST_STRERROR /* Define to 1 when the gnulib module strndup should be tested. */ #undef GNULIB_TEST_STRNDUP /* Define to 1 when the gnulib module strnlen should be tested. */ #undef GNULIB_TEST_STRNLEN /* Define to 1 when the gnulib module symlink should be tested. */ #undef GNULIB_TEST_SYMLINK /* Define to 1 when the gnulib module unsetenv should be tested. */ #undef GNULIB_TEST_UNSETENV /* Define to 1 when the gnulib module vsnprintf should be tested. */ #undef GNULIB_TEST_VSNPRINTF /* Define to 1 when the gnulib module wcrtomb should be tested. */ #undef GNULIB_TEST_WCRTOMB /* Define to 1 when the gnulib module wctob should be tested. */ #undef GNULIB_TEST_WCTOB /* Define to 1 when the gnulib module wctomb should be tested. */ #undef GNULIB_TEST_WCTOMB /* Define to 1 if you have 'alloca' after including , a header that may be supplied by this distribution. */ #undef HAVE_ALLOCA /* Define to 1 if you have and it should be used (not on Ultrix). */ #undef HAVE_ALLOCA_H /* Define to 1 if you have the header file. */ #undef HAVE_BP_SYM_H /* Define to 1 if you have the `btowc' function. */ #undef HAVE_BTOWC /* Define to 1 if you have the Mac OS X function CFLocaleCopyCurrent in the CoreFoundation framework. */ #undef HAVE_CFLOCALECOPYCURRENT /* Define to 1 if you have the Mac OS X function CFPreferencesCopyAppValue in the CoreFoundation framework. */ #undef HAVE_CFPREFERENCESCOPYAPPVALUE /* Define to 1 if you have the declaration of `alarm', and to 0 if you don't. */ #undef HAVE_DECL_ALARM /* Define to 1 if you have the declaration of `clearerr_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_CLEARERR_UNLOCKED /* Define to 1 if you have the declaration of `feof_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FEOF_UNLOCKED /* Define to 1 if you have the declaration of `ferror_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FERROR_UNLOCKED /* Define to 1 if you have the declaration of `fflush_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FFLUSH_UNLOCKED /* Define to 1 if you have the declaration of `fgets_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FGETS_UNLOCKED /* Define to 1 if you have the declaration of `fputc_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FPUTC_UNLOCKED /* Define to 1 if you have the declaration of `fputs_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FPUTS_UNLOCKED /* Define to 1 if you have the declaration of `fread_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FREAD_UNLOCKED /* Define to 1 if you have the declaration of `fwrite_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FWRITE_UNLOCKED /* Define to 1 if you have the declaration of `getchar_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_GETCHAR_UNLOCKED /* Define to 1 if you have the declaration of `getc_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_GETC_UNLOCKED /* Define to 1 if you have the declaration of `getdtablesize', and to 0 if you don't. */ #undef HAVE_DECL_GETDTABLESIZE /* Define to 1 if you have the declaration of `getenv', and to 0 if you don't. */ #undef HAVE_DECL_GETENV /* Define to 1 if you have the declaration of `isblank', and to 0 if you don't. */ #undef HAVE_DECL_ISBLANK /* Define to 1 if you have the declaration of `mbrtowc', and to 0 if you don't. */ #undef HAVE_DECL_MBRTOWC /* Define to 1 if you have the declaration of `mbsinit', and to 0 if you don't. */ #undef HAVE_DECL_MBSINIT /* Define to 1 if you have the declaration of `program_invocation_name', and to 0 if you don't. */ #undef HAVE_DECL_PROGRAM_INVOCATION_NAME /* Define to 1 if you have the declaration of `program_invocation_short_name', and to 0 if you don't. */ #undef HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME /* Define to 1 if you have the declaration of `putchar_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_PUTCHAR_UNLOCKED /* Define to 1 if you have the declaration of `putc_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_PUTC_UNLOCKED /* Define to 1 if you have the declaration of `setenv', and to 0 if you don't. */ #undef HAVE_DECL_SETENV /* Define to 1 if you have the declaration of `sleep', and to 0 if you don't. */ #undef HAVE_DECL_SLEEP /* Define to 1 if you have the declaration of `strerror_r', and to 0 if you don't. */ #undef HAVE_DECL_STRERROR_R /* Define to 1 if you have the declaration of `strncasecmp', and to 0 if you don't. */ #undef HAVE_DECL_STRNCASECMP /* Define to 1 if you have the declaration of `strndup', and to 0 if you don't. */ #undef HAVE_DECL_STRNDUP /* Define to 1 if you have the declaration of `strnlen', and to 0 if you don't. */ #undef HAVE_DECL_STRNLEN /* Define to 1 if you have the declaration of `towlower', and to 0 if you don't. */ #undef HAVE_DECL_TOWLOWER /* Define to 1 if you have the declaration of `unsetenv', and to 0 if you don't. */ #undef HAVE_DECL_UNSETENV /* Define to 1 if you have the declaration of `vsnprintf', and to 0 if you don't. */ #undef HAVE_DECL_VSNPRINTF /* Define to 1 if you have the declaration of `wcrtomb', and to 0 if you don't. */ #undef HAVE_DECL_WCRTOMB /* Define to 1 if you have the declaration of `wctob', and to 0 if you don't. */ #undef HAVE_DECL_WCTOB /* Define to 1 if you have the declaration of `_putenv', and to 0 if you don't. */ #undef HAVE_DECL__PUTENV /* Define to 1 if you have the declaration of `_snprintf', and to 0 if you don't. */ #undef HAVE_DECL__SNPRINTF /* Define to 1 if you have the declaration of `__argv', and to 0 if you don't. */ #undef HAVE_DECL___ARGV /* Define to 1 if you have the header file. */ #undef HAVE_DLFCN_H /* Define to 1 if you have the 'dup2' function. */ #undef HAVE_DUP2 /* Define if you have the declaration of environ. */ #undef HAVE_ENVIRON_DECL /* Define to 1 if you have the header file. */ #undef HAVE_FEATURES_H /* Define to 1 if you have the `flockfile' function. */ #undef HAVE_FLOCKFILE /* Define to 1 if you have the `funlockfile' function. */ #undef HAVE_FUNLOCKFILE /* Define to 1 if you have the `getdtablesize' function. */ #undef HAVE_GETDTABLESIZE /* Define to 1 if you have the `getexecname' function. */ #undef HAVE_GETEXECNAME /* Define to 1 if you have the `getlocalename_l' function. */ #undef HAVE_GETLOCALENAME_L /* Define to 1 if you have the header file. */ #undef HAVE_GETOPT_H /* Define to 1 if you have the `getopt_long_only' function. */ #undef HAVE_GETOPT_LONG_ONLY /* Define to 1 if you have the `getpagesize' function. */ #undef HAVE_GETPAGESIZE /* Define to 1 if you have the `getprogname' function. */ #undef HAVE_GETPROGNAME /* Define to 1 if you have the `gettimeofday' function. */ #undef HAVE_GETTIMEOFDAY /* Define if you have the 'intmax_t' type in or . */ #undef HAVE_INTMAX_T /* Define to 1 if you have the header file. */ #undef HAVE_INTTYPES_H /* Define if exists, doesn't clash with , and declares uintmax_t. */ #undef HAVE_INTTYPES_H_WITH_UINTMAX /* Define to 1 if you have the `isblank' function. */ #undef HAVE_ISBLANK /* Define to 1 if you have the `iswcntrl' function. */ #undef HAVE_ISWCNTRL /* Define to 1 if you have the `iswctype' function. */ #undef HAVE_ISWCTYPE /* Define if you have and nl_langinfo(CODESET). */ #undef HAVE_LANGINFO_CODESET /* Define to 1 if you have the header file. */ #undef HAVE_LANGINFO_H /* Define if your file defines LC_MESSAGES. */ #undef HAVE_LC_MESSAGES /* Define to 1 if you have the header file. */ #undef HAVE_LIBINTL_H /* Has libjpeg */ #undef HAVE_LIBJPEG /* Define to 1 if you have the header file. */ #undef HAVE_LIMITS_H /* Define to 1 if you have the header file. */ #undef HAVE_LINEWRAP_H /* Define to 1 if the system has the type 'long long int'. */ #undef HAVE_LONG_LONG_INT /* Define to 1 if you have the `lstat' function. */ #undef HAVE_LSTAT /* Define to 1 if your system has a GNU libc compatible 'malloc' function, and to 0 otherwise. */ #undef HAVE_MALLOC_GNU /* Define to 1 if you have the header file. */ #undef HAVE_MALLOC_H /* Define if the 'malloc' function is POSIX compliant. */ #undef HAVE_MALLOC_POSIX /* Define to 1 if mmap()'s MAP_ANONYMOUS flag is available after including config.h and . */ #undef HAVE_MAP_ANONYMOUS /* Define to 1 if you have the header file. */ #undef HAVE_MATH_H /* Define to 1 if you have the `mbrtowc' function. */ #undef HAVE_MBRTOWC /* Define to 1 if you have the `mbsinit' function. */ #undef HAVE_MBSINIT /* Define to 1 if declares mbstate_t. */ #undef HAVE_MBSTATE_T /* Define to 1 if you have the header file. */ #undef HAVE_MEMORY_H /* Define to 1 if you have the `mempcpy' function. */ #undef HAVE_MEMPCPY /* Define to 1 if you have the `mprotect' function. */ #undef HAVE_MPROTECT /* Define to 1 on MSVC platforms that have the "invalid parameter handler" concept. */ #undef HAVE_MSVC_INVALID_PARAMETER_HANDLER /* Define to 1 if you have the `newlocale' function. */ #undef HAVE_NEWLOCALE /* Define to 1 if you have the `nl_langinfo' function. */ #undef HAVE_NL_LANGINFO /* Define to 1 if you have the header file. */ #undef HAVE_OS_H /* Define if program_invocation_name is defined */ #undef HAVE_PROGRAM_INVOCATION_NAME /* Define if program_invocation_short_name is defined */ #undef HAVE_PROGRAM_INVOCATION_SHORT_NAME /* Define to 1 if you have the `pstat_getdynamic' function. */ #undef HAVE_PSTAT_GETDYNAMIC /* Define if you have POSIX threads libraries and header files. */ #undef HAVE_PTHREAD /* Define to 1 if you have the `pthread_atfork' function. */ #undef HAVE_PTHREAD_ATFORK /* Define if the defines PTHREAD_MUTEX_RECURSIVE. */ #undef HAVE_PTHREAD_MUTEX_RECURSIVE /* Have PTHREAD_PRIO_INHERIT. */ #undef HAVE_PTHREAD_PRIO_INHERIT /* Define if the POSIX multithreading library has read/write locks. */ #undef HAVE_PTHREAD_RWLOCK /* Define to 1 if you have the `rawmemchr' function. */ #undef HAVE_RAWMEMCHR /* Define to 1 if acosf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ACOSF /* Define to 1 if acosl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ACOSL /* Define to 1 if asinf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ASINF /* Define to 1 if asinl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ASINL /* Define to 1 if atanf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ATANF /* Define to 1 if atanl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ATANL /* Define to 1 if atoll is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ATOLL /* Define to 1 if btowc is declared even after undefining macros. */ #undef HAVE_RAW_DECL_BTOWC /* Define to 1 if canonicalize_file_name is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CANONICALIZE_FILE_NAME /* Define to 1 if cbrt is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CBRT /* Define to 1 if cbrtf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CBRTF /* Define to 1 if cbrtl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CBRTL /* Define to 1 if ceilf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CEILF /* Define to 1 if ceill is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CEILL /* Define to 1 if chdir is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CHDIR /* Define to 1 if chown is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CHOWN /* Define to 1 if copysign is declared even after undefining macros. */ #undef HAVE_RAW_DECL_COPYSIGN /* Define to 1 if copysignf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_COPYSIGNF /* Define to 1 if copysignl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_COPYSIGNL /* Define to 1 if cosf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_COSF /* Define to 1 if coshf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_COSHF /* Define to 1 if cosl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_COSL /* Define to 1 if dprintf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_DPRINTF /* Define to 1 if dup is declared even after undefining macros. */ #undef HAVE_RAW_DECL_DUP /* Define to 1 if dup2 is declared even after undefining macros. */ #undef HAVE_RAW_DECL_DUP2 /* Define to 1 if dup3 is declared even after undefining macros. */ #undef HAVE_RAW_DECL_DUP3 /* Define to 1 if duplocale is declared even after undefining macros. */ #undef HAVE_RAW_DECL_DUPLOCALE /* Define to 1 if endusershell is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ENDUSERSHELL /* Define to 1 if environ is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ENVIRON /* Define to 1 if euidaccess is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EUIDACCESS /* Define to 1 if exp2 is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXP2 /* Define to 1 if exp2f is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXP2F /* Define to 1 if exp2l is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXP2L /* Define to 1 if expf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXPF /* Define to 1 if expl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXPL /* Define to 1 if expm1 is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXPM1 /* Define to 1 if expm1f is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXPM1F /* Define to 1 if expm1l is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXPM1L /* Define to 1 if fabsf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FABSF /* Define to 1 if fabsl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FABSL /* Define to 1 if faccessat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FACCESSAT /* Define to 1 if fchdir is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FCHDIR /* Define to 1 if fchmodat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FCHMODAT /* Define to 1 if fchownat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FCHOWNAT /* Define to 1 if fcntl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FCNTL /* Define to 1 if fdatasync is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FDATASYNC /* Define to 1 if ffs is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FFS /* Define to 1 if ffsl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FFSL /* Define to 1 if ffsll is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FFSLL /* Define to 1 if floorf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FLOORF /* Define to 1 if floorl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FLOORL /* Define to 1 if fma is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FMA /* Define to 1 if fmaf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FMAF /* Define to 1 if fmal is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FMAL /* Define to 1 if fmod is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FMOD /* Define to 1 if fmodf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FMODF /* Define to 1 if fmodl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FMODL /* Define to 1 if fpurge is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FPURGE /* Define to 1 if frexpf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FREXPF /* Define to 1 if frexpl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FREXPL /* Define to 1 if fseeko is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FSEEKO /* Define to 1 if fstat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FSTAT /* Define to 1 if fstatat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FSTATAT /* Define to 1 if fsync is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FSYNC /* Define to 1 if ftello is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FTELLO /* Define to 1 if ftruncate is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FTRUNCATE /* Define to 1 if futimens is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FUTIMENS /* Define to 1 if getcwd is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETCWD /* Define to 1 if getdelim is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETDELIM /* Define to 1 if getdomainname is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETDOMAINNAME /* Define to 1 if getdtablesize is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETDTABLESIZE /* Define to 1 if getgroups is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETGROUPS /* Define to 1 if gethostname is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETHOSTNAME /* Define to 1 if getline is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETLINE /* Define to 1 if getloadavg is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETLOADAVG /* Define to 1 if getlogin is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETLOGIN /* Define to 1 if getlogin_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETLOGIN_R /* Define to 1 if getpagesize is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETPAGESIZE /* Define to 1 if gets is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETS /* Define to 1 if getsubopt is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETSUBOPT /* Define to 1 if gettimeofday is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETTIMEOFDAY /* Define to 1 if getusershell is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETUSERSHELL /* Define to 1 if grantpt is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GRANTPT /* Define to 1 if group_member is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GROUP_MEMBER /* Define to 1 if hypotf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_HYPOTF /* Define to 1 if hypotl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_HYPOTL /* Define to 1 if ilogb is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ILOGB /* Define to 1 if ilogbf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ILOGBF /* Define to 1 if ilogbl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ILOGBL /* Define to 1 if imaxabs is declared even after undefining macros. */ #undef HAVE_RAW_DECL_IMAXABS /* Define to 1 if imaxdiv is declared even after undefining macros. */ #undef HAVE_RAW_DECL_IMAXDIV /* Define to 1 if initstate is declared even after undefining macros. */ #undef HAVE_RAW_DECL_INITSTATE /* Define to 1 if initstate_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_INITSTATE_R /* Define to 1 if isatty is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ISATTY /* Define to 1 if isblank is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ISBLANK /* Define to 1 if iswctype is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ISWCTYPE /* Define to 1 if lchmod is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LCHMOD /* Define to 1 if lchown is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LCHOWN /* Define to 1 if ldexpf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LDEXPF /* Define to 1 if ldexpl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LDEXPL /* Define to 1 if link is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LINK /* Define to 1 if linkat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LINKAT /* Define to 1 if log is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG /* Define to 1 if log10 is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG10 /* Define to 1 if log10f is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG10F /* Define to 1 if log10l is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG10L /* Define to 1 if log1p is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG1P /* Define to 1 if log1pf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG1PF /* Define to 1 if log1pl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG1PL /* Define to 1 if log2 is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG2 /* Define to 1 if log2f is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG2F /* Define to 1 if log2l is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG2L /* Define to 1 if logb is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOGB /* Define to 1 if logbf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOGBF /* Define to 1 if logbl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOGBL /* Define to 1 if logf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOGF /* Define to 1 if logl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOGL /* Define to 1 if lseek is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LSEEK /* Define to 1 if lstat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LSTAT /* Define to 1 if mbrlen is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MBRLEN /* Define to 1 if mbrtowc is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MBRTOWC /* Define to 1 if mbsinit is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MBSINIT /* Define to 1 if mbsnrtowcs is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MBSNRTOWCS /* Define to 1 if mbsrtowcs is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MBSRTOWCS /* Define to 1 if memmem is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MEMMEM /* Define to 1 if mempcpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MEMPCPY /* Define to 1 if memrchr is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MEMRCHR /* Define to 1 if mkdirat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKDIRAT /* Define to 1 if mkdtemp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKDTEMP /* Define to 1 if mkfifo is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKFIFO /* Define to 1 if mkfifoat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKFIFOAT /* Define to 1 if mknod is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKNOD /* Define to 1 if mknodat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKNODAT /* Define to 1 if mkostemp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKOSTEMP /* Define to 1 if mkostemps is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKOSTEMPS /* Define to 1 if mkstemp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKSTEMP /* Define to 1 if mkstemps is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKSTEMPS /* Define to 1 if modf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MODF /* Define to 1 if modff is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MODFF /* Define to 1 if modfl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MODFL /* Define to 1 if nl_langinfo is declared even after undefining macros. */ #undef HAVE_RAW_DECL_NL_LANGINFO /* Define to 1 if openat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_OPENAT /* Define to 1 if pclose is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PCLOSE /* Define to 1 if pipe is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PIPE /* Define to 1 if pipe2 is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PIPE2 /* Define to 1 if popen is declared even after undefining macros. */ #undef HAVE_RAW_DECL_POPEN /* Define to 1 if posix_openpt is declared even after undefining macros. */ #undef HAVE_RAW_DECL_POSIX_OPENPT /* Define to 1 if powf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_POWF /* Define to 1 if pread is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PREAD /* Define to 1 if ptsname is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PTSNAME /* Define to 1 if ptsname_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PTSNAME_R /* Define to 1 if pwrite is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PWRITE /* Define to 1 if qsort_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_QSORT_R /* Define to 1 if random is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RANDOM /* Define to 1 if random_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RANDOM_R /* Define to 1 if rawmemchr is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RAWMEMCHR /* Define to 1 if readlink is declared even after undefining macros. */ #undef HAVE_RAW_DECL_READLINK /* Define to 1 if readlinkat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_READLINKAT /* Define to 1 if realpath is declared even after undefining macros. */ #undef HAVE_RAW_DECL_REALPATH /* Define to 1 if remainder is declared even after undefining macros. */ #undef HAVE_RAW_DECL_REMAINDER /* Define to 1 if remainderf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_REMAINDERF /* Define to 1 if remainderl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_REMAINDERL /* Define to 1 if renameat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RENAMEAT /* Define to 1 if rint is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RINT /* Define to 1 if rintf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RINTF /* Define to 1 if rintl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RINTL /* Define to 1 if rmdir is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RMDIR /* Define to 1 if round is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ROUND /* Define to 1 if roundf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ROUNDF /* Define to 1 if roundl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ROUNDL /* Define to 1 if rpmatch is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RPMATCH /* Define to 1 if secure_getenv is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SECURE_GETENV /* Define to 1 if setenv is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SETENV /* Define to 1 if sethostname is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SETHOSTNAME /* Define to 1 if setlocale is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SETLOCALE /* Define to 1 if setstate is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SETSTATE /* Define to 1 if setstate_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SETSTATE_R /* Define to 1 if setusershell is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SETUSERSHELL /* Define to 1 if sinf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SINF /* Define to 1 if sinhf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SINHF /* Define to 1 if sinl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SINL /* Define to 1 if sleep is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SLEEP /* Define to 1 if snprintf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SNPRINTF /* Define to 1 if sqrtf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SQRTF /* Define to 1 if sqrtl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SQRTL /* Define to 1 if srandom is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SRANDOM /* Define to 1 if srandom_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SRANDOM_R /* Define to 1 if stat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STAT /* Define to 1 if stpcpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STPCPY /* Define to 1 if stpncpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STPNCPY /* Define to 1 if strcasecmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRCASECMP /* Define to 1 if strcasestr is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRCASESTR /* Define to 1 if strchrnul is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRCHRNUL /* Define to 1 if strdup is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRDUP /* Define to 1 if strerror_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRERROR_R /* Define to 1 if strncasecmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRNCASECMP /* Define to 1 if strncat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRNCAT /* Define to 1 if strndup is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRNDUP /* Define to 1 if strnlen is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRNLEN /* Define to 1 if strpbrk is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRPBRK /* Define to 1 if strsep is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRSEP /* Define to 1 if strsignal is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRSIGNAL /* Define to 1 if strtod is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRTOD /* Define to 1 if strtoimax is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRTOIMAX /* Define to 1 if strtok_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRTOK_R /* Define to 1 if strtoll is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRTOLL /* Define to 1 if strtoull is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRTOULL /* Define to 1 if strtoumax is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRTOUMAX /* Define to 1 if strverscmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRVERSCMP /* Define to 1 if symlink is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SYMLINK /* Define to 1 if symlinkat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SYMLINKAT /* Define to 1 if tanf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TANF /* Define to 1 if tanhf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TANHF /* Define to 1 if tanl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TANL /* Define to 1 if tmpfile is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TMPFILE /* Define to 1 if towctrans is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TOWCTRANS /* Define to 1 if trunc is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TRUNC /* Define to 1 if truncf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TRUNCF /* Define to 1 if truncl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TRUNCL /* Define to 1 if ttyname_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TTYNAME_R /* Define to 1 if unlink is declared even after undefining macros. */ #undef HAVE_RAW_DECL_UNLINK /* Define to 1 if unlinkat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_UNLINKAT /* Define to 1 if unlockpt is declared even after undefining macros. */ #undef HAVE_RAW_DECL_UNLOCKPT /* Define to 1 if unsetenv is declared even after undefining macros. */ #undef HAVE_RAW_DECL_UNSETENV /* Define to 1 if usleep is declared even after undefining macros. */ #undef HAVE_RAW_DECL_USLEEP /* Define to 1 if utimensat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_UTIMENSAT /* Define to 1 if vdprintf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_VDPRINTF /* Define to 1 if vsnprintf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_VSNPRINTF /* Define to 1 if wcpcpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCPCPY /* Define to 1 if wcpncpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCPNCPY /* Define to 1 if wcrtomb is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCRTOMB /* Define to 1 if wcscasecmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSCASECMP /* Define to 1 if wcscat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSCAT /* Define to 1 if wcschr is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSCHR /* Define to 1 if wcscmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSCMP /* Define to 1 if wcscoll is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSCOLL /* Define to 1 if wcscpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSCPY /* Define to 1 if wcscspn is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSCSPN /* Define to 1 if wcsdup is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSDUP /* Define to 1 if wcslen is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSLEN /* Define to 1 if wcsncasecmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSNCASECMP /* Define to 1 if wcsncat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSNCAT /* Define to 1 if wcsncmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSNCMP /* Define to 1 if wcsncpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSNCPY /* Define to 1 if wcsnlen is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSNLEN /* Define to 1 if wcsnrtombs is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSNRTOMBS /* Define to 1 if wcspbrk is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSPBRK /* Define to 1 if wcsrchr is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSRCHR /* Define to 1 if wcsrtombs is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSRTOMBS /* Define to 1 if wcsspn is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSSPN /* Define to 1 if wcsstr is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSSTR /* Define to 1 if wcstok is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSTOK /* Define to 1 if wcswidth is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSWIDTH /* Define to 1 if wcsxfrm is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSXFRM /* Define to 1 if wctob is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCTOB /* Define to 1 if wctrans is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCTRANS /* Define to 1 if wctype is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCTYPE /* Define to 1 if wcwidth is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCWIDTH /* Define to 1 if wmemchr is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WMEMCHR /* Define to 1 if wmemcmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WMEMCMP /* Define to 1 if wmemcpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WMEMCPY /* Define to 1 if wmemmove is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WMEMMOVE /* Define to 1 if wmemset is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WMEMSET /* Define to 1 if _Exit is declared even after undefining macros. */ #undef HAVE_RAW_DECL__EXIT /* Define to 1 if you have the `sched_getaffinity' function. */ #undef HAVE_SCHED_GETAFFINITY /* Define to 1 if sched_getaffinity has a glibc compatible declaration. */ #undef HAVE_SCHED_GETAFFINITY_LIKE_GLIBC /* Define to 1 if you have the `sched_getaffinity_np' function. */ #undef HAVE_SCHED_GETAFFINITY_NP /* Define to 1 if you have the header file. */ #undef HAVE_SEARCH_H /* Define to 1 if you have the `setdtablesize' function. */ #undef HAVE_SETDTABLESIZE /* Define to 1 if you have the `setenv' function. */ #undef HAVE_SETENV /* Define to 1 if you have the `setlocale' function. */ #undef HAVE_SETLOCALE /* Define to 1 if 'sig_atomic_t' is a signed integer type. */ #undef HAVE_SIGNED_SIG_ATOMIC_T /* Define to 1 if 'wchar_t' is a signed integer type. */ #undef HAVE_SIGNED_WCHAR_T /* Define to 1 if 'wint_t' is a signed integer type. */ #undef HAVE_SIGNED_WINT_T /* Define to 1 if you have the `sleep' function. */ #undef HAVE_SLEEP /* Define to 1 if you have the `snprintf' function. */ #undef HAVE_SNPRINTF /* Define if the return value of the snprintf function is the number of of bytes (excluding the terminating NUL) that would have been produced if the buffer had been large enough. */ #undef HAVE_SNPRINTF_RETVAL_C99 /* Define to 1 if you have the header file. */ #undef HAVE_STDINT_H /* Define if exists, doesn't clash with , and declares uintmax_t. */ #undef HAVE_STDINT_H_WITH_UINTMAX /* Define to 1 if you have the header file. */ #undef HAVE_STDLIB_H /* Define to 1 if you have the `strcasecmp' function. */ #undef HAVE_STRCASECMP /* Define to 1 if you have the `strchrnul' function. */ #undef HAVE_STRCHRNUL /* Define to 1 if you have the `strerror_r' function. */ #undef HAVE_STRERROR_R /* Define to 1 if you have the header file. */ #undef HAVE_STRINGS_H /* Define to 1 if you have the header file. */ #undef HAVE_STRING_H /* Define to 1 if you have the `strncasecmp' function. */ #undef HAVE_STRNCASECMP /* Define to 1 if you have the `strndup' function. */ #undef HAVE_STRNDUP /* Define to 1 if you have the `strnlen' function. */ #undef HAVE_STRNLEN /* Define to 1 if `decimal_point' is a member of `struct lconv'. */ #undef HAVE_STRUCT_LCONV_DECIMAL_POINT /* Define to 1 if you have the `symlink' function. */ #undef HAVE_SYMLINK /* Define to 1 if you have the `sysctl' function. */ #undef HAVE_SYSCTL /* Define to 1 if you have the header file. */ #undef HAVE_SYSEXITS_H /* Define to 1 if you have the `sysmp' function. */ #undef HAVE_SYSMP /* Define to 1 if you have the header file. */ #undef HAVE_SYS_BITYPES_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_INTTYPES_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_MMAN_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_PARAM_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_PSTAT_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_SOCKET_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_STAT_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_SYSCTL_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_SYSMP_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_TIMEB_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_TIME_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_TYPES_H /* Define to 1 if you have the `towlower' function. */ #undef HAVE_TOWLOWER /* Define to 1 if you have the `tsearch' function. */ #undef HAVE_TSEARCH /* Define to 1 if you have the header file. */ #undef HAVE_UNISTD_H /* Define to 1 if you have the `unsetenv' function. */ #undef HAVE_UNSETENV /* Define to 1 if the system has the type 'unsigned long long int'. */ #undef HAVE_UNSIGNED_LONG_LONG_INT /* Define to 1 if you have the `uselocale' function. */ #undef HAVE_USELOCALE /* Define if you have a global __progname variable */ #undef HAVE_VAR___PROGNAME /* Define to 1 if you have the `vasnprintf' function. */ #undef HAVE_VASNPRINTF /* Define to 1 if you have the `vsnprintf' function. */ #undef HAVE_VSNPRINTF /* Define to 1 if you have the header file. */ #undef HAVE_WCHAR_H /* Define if you have the 'wchar_t' type. */ #undef HAVE_WCHAR_T /* Define to 1 if you have the `wcrtomb' function. */ #undef HAVE_WCRTOMB /* Define to 1 if you have the `wcslen' function. */ #undef HAVE_WCSLEN /* Has wcslib_version */ #undef HAVE_WCSLIB_VERSION /* Define to 1 if you have the `wcsnlen' function. */ #undef HAVE_WCSNLEN /* Define to 1 if you have the `wctob' function. */ #undef HAVE_WCTOB /* Define to 1 if you have the header file. */ #undef HAVE_WCTYPE_H /* Define to 1 if you have the header file. */ #undef HAVE_WINSOCK2_H /* Define if you have the 'wint_t' type. */ #undef HAVE_WINT_T /* Define to 1 if O_NOATIME works. */ #undef HAVE_WORKING_O_NOATIME /* Define to 1 if O_NOFOLLOW works. */ #undef HAVE_WORKING_O_NOFOLLOW /* Define to 1 if you have the header file. */ #undef HAVE_XLOCALE_H /* Define to 1 if the system has the type `_Bool'. */ #undef HAVE__BOOL /* Define to 1 if you have the `_ftime' function. */ #undef HAVE__FTIME /* Define to 1 if you have the `_set_invalid_parameter_handler' function. */ #undef HAVE__SET_INVALID_PARAMETER_HANDLER /* In building, not usage */ #undef IN_GNUASTRO_BUILD /* Define to 1 if 'lstat' dereferences a symlink specified with a trailing slash. */ #undef LSTAT_FOLLOWS_SLASHED_SYMLINK /* Define to the sub-directory where libtool stores uninstalled libraries. */ #undef LT_OBJDIR /* If malloc(0) is != NULL, define this to 1. Otherwise define this to 0. */ #undef MALLOC_0_IS_NONNULL /* Define to a substitute value for mmap()'s MAP_ANONYMOUS flag. */ #undef MAP_ANONYMOUS /* Define if the mbrtowc function does not return (size_t) -2 for empty input. */ #undef MBRTOWC_EMPTY_INPUT_BUG /* Define if the mbrtowc function has the NULL pwc argument bug. */ #undef MBRTOWC_NULL_ARG1_BUG /* Define if the mbrtowc function has the NULL string argument bug. */ #undef MBRTOWC_NULL_ARG2_BUG /* Define if the mbrtowc function does not return 0 for a NUL character. */ #undef MBRTOWC_NUL_RETVAL_BUG /* Define if the mbrtowc function returns a wrong return value. */ #undef MBRTOWC_RETVAL_BUG /* Use GNU style printf and scanf. */ #ifndef __USE_MINGW_ANSI_STDIO # undef __USE_MINGW_ANSI_STDIO #endif /* Define to 1 if open() fails to recognize a trailing slash. */ #undef OPEN_TRAILING_SLASH_BUG /* Name of package */ #undef PACKAGE /* Define to the address where bug reports for this package should be sent. */ #undef PACKAGE_BUGREPORT /* Define to the full name of this package. */ #undef PACKAGE_NAME /* Define to the full name and version of this package. */ #undef PACKAGE_STRING /* Define to the one symbol short name of this package. */ #undef PACKAGE_TARNAME /* Define to the home page for this package. */ #undef PACKAGE_URL /* Define to the version of this package. */ #undef PACKAGE_VERSION /* Define if exists and defines unusable PRI* macros. */ #undef PRI_MACROS_BROKEN /* Define to the type that is the result of default argument promotions of type mode_t. */ #undef PROMOTED_MODE_T /* Define to necessary symbol if this constant uses a non-standard name on your system. */ #undef PTHREAD_CREATE_JOINABLE /* Define if the pthread_in_use() detection is hard. */ #undef PTHREAD_IN_USE_DETECTION_HARD /* Define to l, ll, u, ul, ull, etc., as suitable for constants of type 'ptrdiff_t'. */ #undef PTRDIFF_T_SUFFIX /* Define to 1 if stat needs help when passed a directory name with a trailing slash */ #undef REPLACE_FUNC_STAT_DIR /* Define to 1 if stat needs help when passed a file name with a trailing slash */ #undef REPLACE_FUNC_STAT_FILE /* Define if nl_langinfo exists but is overridden by gnulib. */ #undef REPLACE_NL_LANGINFO /* Define to 1 if strerror(0) does not return a message implying success. */ #undef REPLACE_STRERROR_0 /* Define if vasnprintf exists but is overridden by gnulib. */ #undef REPLACE_VASNPRINTF /* Define to l, ll, u, ul, ull, etc., as suitable for constants of type 'sig_atomic_t'. */ #undef SIG_ATOMIC_T_SUFFIX /* Define as the maximum value of type 'size_t', if the system doesn't define it. */ #ifndef SIZE_MAX # undef SIZE_MAX #endif /* Define to l, ll, u, ul, ull, etc., as suitable for constants of type 'size_t'. */ #undef SIZE_T_SUFFIX /* If using the C implementation of alloca, define if you know the direction of stack growth for your system; otherwise it will be automatically deduced at runtime. STACK_DIRECTION > 0 => grows toward higher addresses STACK_DIRECTION < 0 => grows toward lower addresses STACK_DIRECTION = 0 => direction of growth unknown */ #undef STACK_DIRECTION /* Define to 1 if the `S_IS*' macros in do not work properly. */ #undef STAT_MACROS_BROKEN /* Define to 1 if you have the ANSI C header files. */ #undef STDC_HEADERS /* Define to 1 if strerror_r returns char *. */ #undef STRERROR_R_CHAR_P /* User data dir. */ #undef USERCONFIG_DIR /* Define if the POSIX multithreading library can be used. */ #undef USE_POSIX_THREADS /* Define if references to the POSIX multithreading library should be made weak. */ #undef USE_POSIX_THREADS_WEAK /* Define if the GNU Pth multithreading library can be used. */ #undef USE_PTH_THREADS /* Define if references to the GNU Pth multithreading library should be made weak. */ #undef USE_PTH_THREADS_WEAK /* Define if the old Solaris multithreading library can be used. */ #undef USE_SOLARIS_THREADS /* Define if references to the old Solaris multithreading library should be made weak. */ #undef USE_SOLARIS_THREADS_WEAK /* Enable extensions on AIX 3, Interix. */ #ifndef _ALL_SOURCE # undef _ALL_SOURCE #endif /* Enable general extensions on macOS. */ #ifndef _DARWIN_C_SOURCE # undef _DARWIN_C_SOURCE #endif /* Enable GNU extensions on systems that have them. */ #ifndef _GNU_SOURCE # undef _GNU_SOURCE #endif /* Enable threading extensions on Solaris. */ #ifndef _POSIX_PTHREAD_SEMANTICS # undef _POSIX_PTHREAD_SEMANTICS #endif /* Enable extensions specified by ISO/IEC TS 18661-5:2014. */ #ifndef __STDC_WANT_IEC_60559_ATTRIBS_EXT__ # undef __STDC_WANT_IEC_60559_ATTRIBS_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-1:2014. */ #ifndef __STDC_WANT_IEC_60559_BFP_EXT__ # undef __STDC_WANT_IEC_60559_BFP_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-2:2015. */ #ifndef __STDC_WANT_IEC_60559_DFP_EXT__ # undef __STDC_WANT_IEC_60559_DFP_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-4:2015. */ #ifndef __STDC_WANT_IEC_60559_FUNCS_EXT__ # undef __STDC_WANT_IEC_60559_FUNCS_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-3:2015. */ #ifndef __STDC_WANT_IEC_60559_TYPES_EXT__ # undef __STDC_WANT_IEC_60559_TYPES_EXT__ #endif /* Enable extensions specified by ISO/IEC TR 24731-2:2010. */ #ifndef __STDC_WANT_LIB_EXT2__ # undef __STDC_WANT_LIB_EXT2__ #endif /* Enable extensions specified by ISO/IEC 24747:2009. */ #ifndef __STDC_WANT_MATH_SPEC_FUNCS__ # undef __STDC_WANT_MATH_SPEC_FUNCS__ #endif /* Enable extensions on HP NonStop. */ #ifndef _TANDEM_SOURCE # undef _TANDEM_SOURCE #endif /* Enable X/Open extensions if necessary. HP-UX 11.11 defines mbstate_t only if _XOPEN_SOURCE is defined to 500, regardless of whether compiling with -Ae or -D_HPUX_SOURCE=1. */ #ifndef _XOPEN_SOURCE # undef _XOPEN_SOURCE #endif /* Enable general extensions on Solaris. */ #ifndef __EXTENSIONS__ # undef __EXTENSIONS__ #endif /* Define if the native Windows multithreading API can be used. */ #undef USE_WINDOWS_THREADS /* Version number of package */ #undef VERSION /* Define to 1 if unsetenv returns void instead of int. */ #undef VOID_UNSETENV /* Define to l, ll, u, ul, ull, etc., as suitable for constants of type 'wchar_t'. */ #undef WCHAR_T_SUFFIX /* Define to l, ll, u, ul, ull, etc., as suitable for constants of type 'wint_t'. */ #undef WINT_T_SUFFIX /* Define WORDS_BIGENDIAN to 1 if your processor stores words with the most significant byte first (like Motorola and SPARC, unlike Intel). */ #if defined AC_APPLE_UNIVERSAL_BUILD # if defined __BIG_ENDIAN__ # define WORDS_BIGENDIAN 1 # endif #else # ifndef WORDS_BIGENDIAN # undef WORDS_BIGENDIAN # endif #endif /* Enable large inode numbers on Mac OS X 10.5. */ #undef _DARWIN_USE_64_BIT_INODE /* Number of bits in a file offset, on hosts where this is settable. */ #undef _FILE_OFFSET_BITS /* Define to 1 if Gnulib overrides 'struct stat' on Windows so that struct stat.st_size becomes 64-bit. */ #undef _GL_WINDOWS_64_BIT_ST_SIZE /* Define for large files, on AIX-style hosts. */ #undef _LARGE_FILES /* Define to 1 on Solaris. */ #undef _LCONV_C99 /* Define to 1 if on MINIX. */ #undef _MINIX /* Define to 1 to make NetBSD features available. MINIX 3 needs this. */ #undef _NETBSD_SOURCE /* The _Noreturn keyword of C11. */ #if ! (defined _Noreturn \ || (defined __STDC_VERSION__ && 201112 <= __STDC_VERSION__)) # if (3 <= __GNUC__ || (__GNUC__ == 2 && 8 <= __GNUC_MINOR__) \ || 0x5110 <= __SUNPRO_C) # define _Noreturn __attribute__ ((__noreturn__)) # elif defined _MSC_VER && 1200 <= _MSC_VER # define _Noreturn __declspec (noreturn) # else # define _Noreturn # endif #endif /* Define to 2 if the system does not provide POSIX.1 features except with this defined. */ #undef _POSIX_1_SOURCE /* Define to 1 if you need to in order for 'stat' and other things to work. */ #undef _POSIX_SOURCE /* Define if you want to include , so that it consistently overrides 's RE_DUP_MAX. */ #undef _REGEX_INCLUDE_LIMITS_H /* Define if you want regoff_t to be at least as wide POSIX requires. */ #undef _REGEX_LARGE_OFFSETS /* Define to rpl_ if the getopt replacement functions and variables should be used. */ #undef __GETOPT_PREFIX /* Define to 1 if the system predates C++11. */ #undef __STDC_CONSTANT_MACROS /* Define to 1 if the system predates C++11. */ #undef __STDC_LIMIT_MACROS /* Please see the Gnulib manual for how to use these macros. Suppress extern inline with HP-UX cc, as it appears to be broken; see . Suppress extern inline with Sun C in standards-conformance mode, as it mishandles inline functions that call each other. E.g., for 'inline void f (void) { } inline void g (void) { f (); }', c99 incorrectly complains 'reference to static identifier "f" in extern inline function'. This bug was observed with Sun C 5.12 SunOS_i386 2011/11/16. Suppress extern inline (with or without __attribute__ ((__gnu_inline__))) on configurations that mistakenly use 'static inline' to implement functions or macros in standard C headers like . For example, if isdigit is mistakenly implemented via a static inline function, a program containing an extern inline function that calls isdigit may not work since the C standard prohibits extern inline functions from calling static functions. This bug is known to occur on: OS X 10.8 and earlier; see: http://lists.gnu.org/archive/html/bug-gnulib/2012-12/msg00023.html DragonFly; see http://muscles.dragonflybsd.org/bulk/bleeding-edge-potential/latest-per-pkg/ah-tty-0.3.12.log FreeBSD; see: http://lists.gnu.org/archive/html/bug-gnulib/2014-07/msg00104.html OS X 10.9 has a macro __header_inline indicating the bug is fixed for C and for clang but remains for g++; see . Assume DragonFly and FreeBSD will be similar. */ #if (((defined __APPLE__ && defined __MACH__) \ || defined __DragonFly__ || defined __FreeBSD__) \ && (defined __header_inline \ ? (defined __cplusplus && defined __GNUC_STDC_INLINE__ \ && ! defined __clang__) \ : ((! defined _DONT_USE_CTYPE_INLINE_ \ && (defined __GNUC__ || defined __cplusplus)) \ || (defined _FORTIFY_SOURCE && 0 < _FORTIFY_SOURCE \ && defined __GNUC__ && ! defined __cplusplus)))) # define _GL_EXTERN_INLINE_STDHEADER_BUG #endif #if ((__GNUC__ \ ? defined __GNUC_STDC_INLINE__ && __GNUC_STDC_INLINE__ \ : (199901L <= __STDC_VERSION__ \ && !defined __HP_cc \ && !defined __PGI \ && !(defined __SUNPRO_C && __STDC__))) \ && !defined _GL_EXTERN_INLINE_STDHEADER_BUG) # define _GL_INLINE inline # define _GL_EXTERN_INLINE extern inline # define _GL_EXTERN_INLINE_IN_USE #elif (2 < __GNUC__ + (7 <= __GNUC_MINOR__) && !defined __STRICT_ANSI__ \ && !defined _GL_EXTERN_INLINE_STDHEADER_BUG) # if defined __GNUC_GNU_INLINE__ && __GNUC_GNU_INLINE__ /* __gnu_inline__ suppresses a GCC 4.2 diagnostic. */ # define _GL_INLINE extern inline __attribute__ ((__gnu_inline__)) # else # define _GL_INLINE extern inline # endif # define _GL_EXTERN_INLINE extern # define _GL_EXTERN_INLINE_IN_USE #else # define _GL_INLINE static _GL_UNUSED # define _GL_EXTERN_INLINE static _GL_UNUSED #endif /* In GCC 4.6 (inclusive) to 5.1 (exclusive), suppress bogus "no previous prototype for 'FOO'" and "no previous declaration for 'FOO'" diagnostics, when FOO is an inline function in the header; see and . */ #if __GNUC__ == 4 && 6 <= __GNUC_MINOR__ # if defined __GNUC_STDC_INLINE__ && __GNUC_STDC_INLINE__ # define _GL_INLINE_HEADER_CONST_PRAGMA # else # define _GL_INLINE_HEADER_CONST_PRAGMA \ _Pragma ("GCC diagnostic ignored \"-Wsuggest-attribute=const\"") # endif # define _GL_INLINE_HEADER_BEGIN \ _Pragma ("GCC diagnostic push") \ _Pragma ("GCC diagnostic ignored \"-Wmissing-prototypes\"") \ _Pragma ("GCC diagnostic ignored \"-Wmissing-declarations\"") \ _GL_INLINE_HEADER_CONST_PRAGMA # define _GL_INLINE_HEADER_END \ _Pragma ("GCC diagnostic pop") #else # define _GL_INLINE_HEADER_BEGIN # define _GL_INLINE_HEADER_END #endif /* Define to `__inline__' or `__inline' if that's what the C compiler calls it, or to nothing if 'inline' is not supported under any name. */ #ifndef __cplusplus #undef inline #endif /* Define to long or long long if and don't define. */ #undef intmax_t /* Work around a bug in Apple GCC 4.0.1 build 5465: In C99 mode, it supports the ISO C 99 semantics of 'extern inline' (unlike the GNU C semantics of earlier versions), but does not display it by setting __GNUC_STDC_INLINE__. __APPLE__ && __MACH__ test for Mac OS X. __APPLE_CC__ tests for the Apple compiler and its version. __STDC_VERSION__ tests for the C99 mode. */ #if defined __APPLE__ && defined __MACH__ && __APPLE_CC__ >= 5465 && !defined __cplusplus && __STDC_VERSION__ >= 199901L && !defined __GNUC_STDC_INLINE__ # define __GNUC_STDC_INLINE__ 1 #endif /* Define to a type if does not define. */ #undef mbstate_t /* Define to `int' if does not define. */ #undef mode_t /* Define to the type of st_nlink in struct stat, or a supertype. */ #undef nlink_t /* Define to `int' if does not define. */ #undef pid_t /* Define as the type of the result of subtracting two pointers, if the system doesn't define it. */ #undef ptrdiff_t /* Define to rpl_re_comp if the replacement should be used. */ #undef re_comp /* Define to rpl_re_compile_fastmap if the replacement should be used. */ #undef re_compile_fastmap /* Define to rpl_re_compile_pattern if the replacement should be used. */ #undef re_compile_pattern /* Define to rpl_re_exec if the replacement should be used. */ #undef re_exec /* Define to rpl_re_match if the replacement should be used. */ #undef re_match /* Define to rpl_re_match_2 if the replacement should be used. */ #undef re_match_2 /* Define to rpl_re_search if the replacement should be used. */ #undef re_search /* Define to rpl_re_search_2 if the replacement should be used. */ #undef re_search_2 /* Define to rpl_re_set_registers if the replacement should be used. */ #undef re_set_registers /* Define to rpl_re_set_syntax if the replacement should be used. */ #undef re_set_syntax /* Define to rpl_re_syntax_options if the replacement should be used. */ #undef re_syntax_options /* Define to rpl_regcomp if the replacement should be used. */ #undef regcomp /* Define to rpl_regerror if the replacement should be used. */ #undef regerror /* Define to rpl_regexec if the replacement should be used. */ #undef regexec /* Define to rpl_regfree if the replacement should be used. */ #undef regfree /* Define to the equivalent of the C99 'restrict' keyword, or to nothing if this is not supported. 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@GNULIB_DPRINTF@ GNULIB_DUP = @GNULIB_DUP@ GNULIB_DUP2 = @GNULIB_DUP2@ GNULIB_DUP3 = @GNULIB_DUP3@ GNULIB_DUPLOCALE = @GNULIB_DUPLOCALE@ GNULIB_ENVIRON = @GNULIB_ENVIRON@ GNULIB_EUIDACCESS = @GNULIB_EUIDACCESS@ GNULIB_EXP2 = @GNULIB_EXP2@ GNULIB_EXP2F = @GNULIB_EXP2F@ GNULIB_EXP2L = @GNULIB_EXP2L@ GNULIB_EXPF = @GNULIB_EXPF@ GNULIB_EXPL = @GNULIB_EXPL@ GNULIB_EXPM1 = @GNULIB_EXPM1@ GNULIB_EXPM1F = @GNULIB_EXPM1F@ GNULIB_EXPM1L = @GNULIB_EXPM1L@ GNULIB_FABSF = @GNULIB_FABSF@ GNULIB_FABSL = @GNULIB_FABSL@ GNULIB_FACCESSAT = @GNULIB_FACCESSAT@ GNULIB_FCHDIR = @GNULIB_FCHDIR@ GNULIB_FCHMODAT = @GNULIB_FCHMODAT@ GNULIB_FCHOWNAT = @GNULIB_FCHOWNAT@ GNULIB_FCLOSE = @GNULIB_FCLOSE@ GNULIB_FCNTL = @GNULIB_FCNTL@ GNULIB_FDATASYNC = @GNULIB_FDATASYNC@ GNULIB_FDOPEN = @GNULIB_FDOPEN@ GNULIB_FFLUSH = @GNULIB_FFLUSH@ GNULIB_FFS = @GNULIB_FFS@ GNULIB_FFSL = @GNULIB_FFSL@ GNULIB_FFSLL = @GNULIB_FFSLL@ GNULIB_FGETC = @GNULIB_FGETC@ GNULIB_FGETS = @GNULIB_FGETS@ GNULIB_FLOOR = @GNULIB_FLOOR@ GNULIB_FLOORF = @GNULIB_FLOORF@ GNULIB_FLOORL = @GNULIB_FLOORL@ GNULIB_FMA = @GNULIB_FMA@ GNULIB_FMAF = @GNULIB_FMAF@ GNULIB_FMAL = @GNULIB_FMAL@ GNULIB_FMOD = @GNULIB_FMOD@ GNULIB_FMODF = @GNULIB_FMODF@ GNULIB_FMODL = @GNULIB_FMODL@ GNULIB_FOPEN = @GNULIB_FOPEN@ GNULIB_FPRINTF = @GNULIB_FPRINTF@ GNULIB_FPRINTF_POSIX = @GNULIB_FPRINTF_POSIX@ GNULIB_FPURGE = @GNULIB_FPURGE@ GNULIB_FPUTC = @GNULIB_FPUTC@ GNULIB_FPUTS = @GNULIB_FPUTS@ GNULIB_FREAD = @GNULIB_FREAD@ GNULIB_FREOPEN = @GNULIB_FREOPEN@ GNULIB_FREXP = @GNULIB_FREXP@ GNULIB_FREXPF = @GNULIB_FREXPF@ GNULIB_FREXPL = @GNULIB_FREXPL@ GNULIB_FSCANF = @GNULIB_FSCANF@ GNULIB_FSEEK = @GNULIB_FSEEK@ GNULIB_FSEEKO = @GNULIB_FSEEKO@ GNULIB_FSTAT = @GNULIB_FSTAT@ GNULIB_FSTATAT = @GNULIB_FSTATAT@ GNULIB_FSYNC = @GNULIB_FSYNC@ GNULIB_FTELL = @GNULIB_FTELL@ GNULIB_FTELLO = @GNULIB_FTELLO@ GNULIB_FTRUNCATE = @GNULIB_FTRUNCATE@ GNULIB_FUTIMENS = @GNULIB_FUTIMENS@ GNULIB_FWRITE = @GNULIB_FWRITE@ GNULIB_GETC = @GNULIB_GETC@ GNULIB_GETCHAR = @GNULIB_GETCHAR@ GNULIB_GETCWD = @GNULIB_GETCWD@ GNULIB_GETDELIM = @GNULIB_GETDELIM@ GNULIB_GETDOMAINNAME = @GNULIB_GETDOMAINNAME@ GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = 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then \ echo; \ echo "==================================================================="; \ echo "==================================================================="; \ echo "Gnuastro $(VERSION), was successfully built."; \ echo "Please check the build on your system by running:"; \ echo; \ echo " make check"; \ echo; \ echo "(Check faster on N threads with 'make check -jN'.)"; \ echo "(The following \"Leaving directory\" notices can be ignored.)"; \ echo "==================================================================="; \ echo "==================================================================="; \ echo; \ fi check-local: @if [ x$(GUIDEMESSAGE) = xyes ]; then \ echo; \ echo "==================================================================="; \ echo "==================================================================="; \ echo "Your build of Gnuastro $(VERSION) didn't fail on any tests."; \ echo "To install Gnuastro, please run the commands below:"; \ echo; \ if [ ! -w $(prefix) ] ; then \ echo "(NOTE: As the user $$USER, you don't have writing permissions"; \ echo "in \"$(prefix)\". To install Gnuastro there, you must get "; \ echo "privileges first, as described below. If you can't, configure "; \ echo "Gnuastro again, for example: \"./configure --prefix ~/.local\".)"; \ echo; \ echo " sudo make install"; \ echo "or"; \ echo " su"; \ fi; \ echo " make install"; \ if [ ! -w $(prefix) ] ; then \ echo " exit"; \ fi; \ echo; \ echo "(The following \"Leaving directory\" notices can be ignored.)"; \ echo "==================================================================="; \ echo "==================================================================="; \ echo; \ fi install-exec-local: @if [ x$(GUIDEMESSAGE) = xyes ]; then \ echo; \ echo "==================================================================="; \ echo "==================================================================="; \ echo " , , "; \ echo " / \ "; \ echo " ((__-^^-,-^^-__)) Congratulations!"; \ echo " \`-_---' \`---_-' GNU Astronomy Utilities (Gnuastro),"; \ echo " \`--|o\` 'o|--' Version $(VERSION)"; \ echo " \ \` / "; \ echo " ): :( Successfully installed on this system."; \ echo " :o_o: "; \ echo " \"-\" "; \ echo; \ echo "More information Command to run "; \ echo "---------------- -------------- "; \ echo "Complete official Gnuastro book: ' info gnuastro '"; \ echo "Entertaining tutorials: ' info gnuastro Tutorials '"; \ echo "Dedicated help mailing list: ' info help-gnuastro '"; \ echo "Instructions for reporting bugs: ' info bug-gnuastro '"; \ echo "Effectively use Info: ' info info '"; \ echo; \ echo; \ echo "Environment variables to check: "; \ echo " - '$(prefix)/bin' in PATH."; \ echo "(for an intro, run 'info gnuastro \"Installation directory\"')"; \ echo; \ echo; \ echo "To stay up to date with future releases, please subscribe to: "; \ echo " https://lists.gnu.org/mailman/listinfo/info-gnuastro"; \ echo; \ echo; \ echo "(The following lines can be ignored.)"; \ echo "==================================================================="; \ echo "==================================================================="; \ echo; \ fi $(top_srcdir)/.version: $(top_srcdir)/configure echo $(VERSION) > $@-t && mv $@-t $@ $(top_srcdir)/AUTHORS: $(top_srcdir)/.version $(top_srcdir)/genauthors $(top_srcdir) dist-hook: $(top_srcdir)/AUTHORS echo $(VERSION) > $(distdir)/.tarball-version # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: gnuastro-0.2.33-8a3b/README0000644000175000017500000002232312774314223012004 00000000000000GNU Astronomy Utilities ======================= GNU Astronomy Utilities (Gnuastro) is an official GNU package of programs and a library functions for astronomical data manipulation and analysis. The programs are run directory on the operating system's command-line enabling easy and efficient operation combined with other installed programs in shell scripts or Makefiles. The libraries are also usable in C and C++ programs. The full package comes with a comprehensive book or documentation in various formats (plain text, info, PDF and HTML): http://www.gnu.org/software/gnuastro/manual/ The Gnuastro book explains all the mathematical, physical and even historical concepts (when necessary) for effective usage of all the programs and libraries along with short examples for each program and full descriptions of all their options (in the "Invoking ProgramName' sections). There is also a separate chapter devoted to tutorials for effectively use Gnuastro combined with other software already available on your Unix-like operating system (see Chapter 2). If you have already installed gnuastro, you can read the full book by running the following command. You can go through the whole book by pressing the 'SPACE' key, and leave the Info environment at any time by pressing 'q' key. See the "Getting help" section below (in this file) or in the book for more. info gnuastro The programs released in version 0.2 are listed below followed by their executable name in parenthesis and a short description. This list is ordered alphabetically. In the book, they are grouped and ordered by context under categories/chapters. - Arithmetic (astarithmetic): For arithmetic operations on multiple (theoretically unlimited) number of datasets (images). It has a large and growing set of arithmetic, mathematical, and even statistical operators (for example +, -, *, /, sqrt, log, min, average, median). - ConvertType (astconvertt): Convert astronomical data files (FITS or IMH) to and from several other standard image and data formats, for example TXT, JPEG, EPS or PDF. - Convolve (astconvolve): Convolve (blur or smooth) data with a given kernel in spatial and frequency domain on multiple threads. Convolve can also do de-convolution to find the appropriate kernel to PSF-match two images. - CosmicCalculator (astconvolve): Do cosmological calculations, for example the luminosity distance, distance modulus, comoving volume and many more. - Header (astheader): Print and manipulate the header data of a FITS file. - ImageCrop (astimgcrop): Crop region(s) from an image and stitch several images if necessary. Inputs can be in pixel coordinates or world coordinates. - ImageStatistics (astimgstat): Get pixel statistics and save histogram and cumulative frequency plots. - ImageWarp (astimgwarp): Warp image to new pixel grid. Any projective transformation or Homography can be applied to the input images. - MakeCatalog (astmkcatalog): Make catalog of labeled image (output of NoiseChisel). The catalogs are highly customizable and adding new calculations/columns is very streightforward. - MakeNoise (astmknoise): Make (add) noise to an image, with a large set of random number generators and any seed. - MakeProfiles (astmkprof): Make mock 2D profiles in an image. The central regions of radial profiles are made with a configurable 2D Monte Carlo integration. It can also build the profiles on an over-sampled image. - NoiseChisel (astnoisechisel): Detect and segment signal in noise. It uses a technique to detect very faint and diffuse, irregularly shaped signal in noise (galaxies in the sky), using thresholds that are below the Sky value (see arXiv:1505.01664). - SubtractSky (astsubtractsky): Find and subtract sky value by comparing the mode and median on a mesh grid. - Table (asttable): convert FITS binary and ASCII tables into other such tables, or print them on the command-line, or save them in a plain text file. Output columns can also be determined by number or regular expression matching of column names. All the programs share the same basic command-line user interface and a set of common options for the comfort of both the users and developers. Gnuastro is written to comply fully with the GNU coding standards so it integrates finely with the GNU/Linux operating system and Unix-like operating systems in general. This also enables astronomers to expect a fully familiar experience in the source code, building, installing and command line user interaction that they have seen in all the other GNU software that they use. Behind the scenes, Gnuastro comes with a very robust infra-structure enabling easy addition of new programs and new features to existing programs and a full chapter devoted to explaining how to develop most effectively (see the "Developing" chapter). Please join us in developing this comprehensive and low level set of tools for astronomical data manipulation and analysis. The copyright owner of Gnuastro is the Free Software Foundation to guarantee its freedom in the future, and not any particular astronomer or astronomical project, or astronomical institution, so please join us and feel free to use it in your research. Installing Gnuastro ------------------- The mandatory dependencies which are required to install Gnuastro from the tarball are listed below. See the "Dependencies" section of the book for their detailed installation guides and optional dependencies to enable extra features. If you have just cloned Gnuastro and want to install from the version controlled source, please read the 'README-hacking' file (not available in the tarball) or the "Bootstrapping dependencies" subsection of the manual before continuing. - GNU Scientific Library (GSL): https://www.gnu.org/software/gsl/ - CFITSIO: http://heasarc.gsfc.nasa.gov/fitsio/ - WCSLIB: http://www.atnf.csiro.au/people/mcalabre/WCS/ The most recent stable Gnuastro release can be downloaded from the following link. Please see the "Downloading the source" section of the Gnuastro book for a more complete discussion of your download options. http://ftp.gnu.org/gnu/gnuastro/gnuastro-latest.tar.gz Unpacking, configuring, building, checking and installing Gnuastro follows the standard GNU Build system as shown below. After the './configure' command, Gnuastro will print messages upon the successful completion of each step, giving further information and suggestions for the next steps. tar xf gnuastro-latest.tar.gz # Also works for `tar.lz' files cd gnuastro-0.1 ./configure make make check sudo make install See the "Build and install" section of the book for more information. Also, see the 'INSTALL' file which is distributed with this file for a standard (very comprehensive and general) review of the GNU build and install methods. The 'INSTALL' file is shared in many software packages, so reading it once in any package is enough to help you greatly customize your build of a very large collection of Free and Open Source (FOSS) software. Getting help ------------ To access the appropriate section of the Gnuastro book/documentation from your command-line (in the middle of your work, without distracting your self by having to move your hand off the keyboard), please run any of the following two commands. Note that you can leave the Info environment by pressing the key `q'. info ProgramName # For example 'info NoiseChisel' info astprogname # For example 'info astnoisechisel' The Info environment is great for easily reading of the complete documentation of many software packages, not just Gnuastro. It can greatly enhance your life/work in the Unix-like operating systems. If you are not familiar with it, please run the following command and read through it (it is short and only takes about an hour, so we strongly recommend it): info info To immediately get a short list of each programs's options and a short explanation of each, please run: astprogname --help # For example 'astnoisechisel --help' Ultimately you can send a mail to 'help-gnuastro@gnu.org' to get help in installing or using Gnuastro. Some Gnuastro developers and active users are subscribed to this list and are ready to help you in using these programs. Reporting bugs -------------- The most effective way to report bugs is explained in the "Report a bug" section of the documentation, after installation, you can read it by running (leave the Info environment by pressing the `q' key afterwards): info bug-gnuastro In short, you can send a mail to 'bug-gnuastro@gnu.org', or submit a report in the link below (the latter is recommended): https://savannah.gnu.org/support/?func=additem&group=gnuastro In any case, please be very descriptive and give the exact command that produced the bug, we will be able to solve it faster and more effectively if we can reproduce it after your first report. The list of previous bugs along with their status can be seen here https://savannah.gnu.org/bugs/?group=gnuastro Have a look in the link above to see if your problem has already been addressed. 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"invalid value of canonical build" "$LINENO" 5;; esac build=$ac_cv_build ac_save_IFS=$IFS; IFS='-' set x $ac_cv_build shift build_cpu=$1 build_vendor=$2 shift; shift # Remember, the first character of IFS is used to create $*, # except with old shells: build_os=$* IFS=$ac_save_IFS case $build_os in *\ *) build_os=`echo "$build_os" | sed 's/ /-/g'`;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking host system type" >&5 $as_echo_n "checking host system type... " >&6; } if ${ac_cv_host+:} false; then : $as_echo_n "(cached) " >&6 else if test "x$host_alias" = x; then ac_cv_host=$ac_cv_build else ac_cv_host=`$SHELL "$ac_aux_dir/config.sub" $host_alias` || as_fn_error $? "$SHELL $ac_aux_dir/config.sub $host_alias failed" "$LINENO" 5 fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_host" >&5 $as_echo "$ac_cv_host" >&6; } case $ac_cv_host in *-*-*) ;; *) as_fn_error $? "invalid value of canonical host" "$LINENO" 5;; esac host=$ac_cv_host ac_save_IFS=$IFS; IFS='-' set x $ac_cv_host shift host_cpu=$1 host_vendor=$2 shift; shift # Remember, the first character of IFS is used to create $*, # except with old shells: host_os=$* IFS=$ac_save_IFS case $host_os in *\ *) host_os=`echo "$host_os" | sed 's/ /-/g'`;; esac # IEEE behaviour is the default on all CPUs except Alpha and SH # (according to the test results of Bruno Haible's ieeefp/fenv_default.m4 # and the GCC 4.1.2 manual). case "$host_cpu" in alpha*) # On Alpha systems, a compiler option provides the behaviour. # See the ieee(3) manual page, also available at # if test -n "$GCC"; then # GCC has the option -mieee. # For full IEEE compliance (rarely needed), use option -mieee-with-inexact. CPPFLAGS="$CPPFLAGS -mieee" else # Compaq (ex-DEC) C has the option -ieee, equivalent to -ieee_with_no_inexact. # For full IEEE compliance (rarely needed), use option -ieee_with_inexact. 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" >&6; } if ${ac_cv_sys_large_files+:} false; then : $as_echo_n "(cached) " >&6 else while :; do cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include /* Check that off_t can represent 2**63 - 1 correctly. We can't simply define LARGE_OFF_T to be 9223372036854775807, since some C++ compilers masquerading as C compilers incorrectly reject 9223372036854775807. */ #define LARGE_OFF_T (((off_t) 1 << 62) - 1 + ((off_t) 1 << 62)) int off_t_is_large[(LARGE_OFF_T % 2147483629 == 721 && LARGE_OFF_T % 2147483647 == 1) ? 1 : -1]; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_sys_large_files=no; break fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #define _LARGE_FILES 1 #include /* Check that off_t can represent 2**63 - 1 correctly. We can't simply define LARGE_OFF_T to be 9223372036854775807, since some C++ compilers masquerading as C compilers incorrectly reject 9223372036854775807. */ #define LARGE_OFF_T (((off_t) 1 << 62) - 1 + ((off_t) 1 << 62)) int off_t_is_large[(LARGE_OFF_T % 2147483629 == 721 && LARGE_OFF_T % 2147483647 == 1) ? 1 : -1]; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_sys_large_files=1; break fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext ac_cv_sys_large_files=unknown break done fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_sys_large_files" >&5 $as_echo "$ac_cv_sys_large_files" >&6; } case $ac_cv_sys_large_files in #( no | unknown) ;; *) cat >>confdefs.h <<_ACEOF #define _LARGE_FILES $ac_cv_sys_large_files _ACEOF ;; esac rm -rf conftest* fi $as_echo "#define _DARWIN_USE_64_BIT_INODE 1" >>confdefs.h fi # Check whether --enable-threads was given. if test "${enable_threads+set}" = set; then : enableval=$enable_threads; gl_use_threads=$enableval else if test -n "$gl_use_threads_default"; then gl_use_threads="$gl_use_threads_default" else case "$host_os" in osf*) gl_use_threads=no ;; cygwin*) case `uname -r` in 1.[0-5].*) gl_use_threads=no ;; *) gl_use_threads=yes ;; esac ;; *) gl_use_threads=yes ;; esac fi fi if test "$gl_use_threads" = yes || test "$gl_use_threads" = posix; then # For using : case "$host_os" in osf*) # On OSF/1, the compiler needs the flag -D_REENTRANT so that it # groks . cc also understands the flag -pthread, but # we don't use it because 1. gcc-2.95 doesn't understand -pthread, # 2. putting a flag into CPPFLAGS that has an effect on the linker # causes the AC_LINK_IFELSE test below to succeed unexpectedly, # leading to wrong values of LIBTHREAD and LTLIBTHREAD. CPPFLAGS="$CPPFLAGS -D_REENTRANT" ;; esac # Some systems optimize for single-threaded programs by default, and # need special flags to disable these optimizations. 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Code from module errno: # Code from module errno-tests: # Code from module error: # Code from module extensions: # Code from module extern-inline: # Code from module fcntl-h: # Code from module fcntl-h-tests: # Code from module fd-hook: # Code from module fdl: # Code from module fdopen: # Code from module fdopen-tests: # Code from module fgetc-tests: # Code from module flexmember: # Code from module float: # Code from module float-tests: # Code from module fpieee: # Code from module fpucw: # Code from module fputc-tests: # Code from module fread-tests: # Code from module fstat: # Code from module fstat-tests: # Code from module fwrite-tests: # Code from module gendocs: # Code from module getcwd-lgpl: # Code from module getcwd-lgpl-tests: # Code from module getdtablesize: # Code from module getdtablesize-tests: # Code from module getopt-gnu: # Code from module getopt-posix: # Code from module getopt-posix-tests: # Code from module getpagesize: # Code from module getprogname: # Code from module getprogname-tests: # Code from module gettext-h: # Code from module gettimeofday: # Code from module gettimeofday-tests: # Code from module git-version-gen: # Code from module hard-locale: # Code from module havelib: # Code from module ignore-value: # Code from module ignore-value-tests: # Code from module include_next: # Code from module intprops: # Code from module intprops-tests: # Code from module inttypes: # Code from module inttypes-incomplete: # Code from module inttypes-tests: # Code from module langinfo: # Code from module langinfo-tests: # Code from module largefile: # Code from module limits-h: # Code from module limits-h-tests: # Code from module localcharset: # Code from module locale: # Code from module locale-tests: # Code from module localeconv: # Code from module localeconv-tests: # Code from module localename: # Code from module localename-tests: # Code from module lock: # Code from module lock-tests: # Code from module lstat: # Code from module lstat-tests: # Code from module malloc-gnu: # Code from module malloc-gnu-tests: # Code from module malloc-posix: # Code from module malloca: # Code from module malloca-tests: # Code from module math: # Code from module math-tests: # Code from module mbrtowc: # Code from module mbrtowc-tests: # Code from module mbsinit: # Code from module mbsinit-tests: # Code from module mbtowc: # Code from module memchr: # Code from module memchr-tests: # Code from module mempcpy: # Code from module msvc-inval: # Code from module msvc-nothrow: # Code from module multiarch: # Code from module nl_langinfo: # Code from module nl_langinfo-tests: # Code from module nocrash: # Code from module nproc: # Code from module open: # Code from module open-tests: # Code from module pathmax: # Code from module pathmax-tests: # Code from module putenv: # Code from module rawmemchr: # Code from module rawmemchr-tests: # Code from module regex: # Code from module regex-tests: # Code from module same-inode: # Code from module setenv: # Code from module setenv-tests: # Code from module setlocale: # Code from module setlocale-tests: # Code from module size_max: # Code from module sleep: # Code from module sleep-tests: # Code from module snippet/_Noreturn: # Code from module snippet/arg-nonnull: # Code from module snippet/c++defs: # Code from module snippet/warn-on-use: # Code from module ssize_t: # Code from module stat: # Code from module stat-tests: # Code from module stdalign: # Code from module stdalign-tests: # Code from module stdbool: # Code from module stdbool-tests: # Code from module stddef: # Code from module stddef-tests: # Code from module stdint: # Code from module stdint-tests: # Code from module stdio: # Code from module stdio-tests: # Code from module stdlib: # Code from module stdlib-tests: # Code from module strcase: # Code from module strchrnul: # Code from module strchrnul-tests: # Code from module streq: # Code from module strerror: # Code from module strerror-override: # Code from module strerror-tests: # Code from module string: # Code from module string-tests: # Code from module strings: # Code from module strings-tests: # Code from module strndup: # Code from module strnlen: # Code from module strnlen-tests: # Code from module symlink: # Code from module symlink-tests: # Code from module sys_stat: # Code from module sys_stat-tests: # Code from module sys_time: # Code from module sys_time-tests: # Code from module sys_types: # Code from module sys_types-tests: # Code from module sysexits: # Code from module sysexits-tests: # Code from module test-framework-sh: # Code from module test-framework-sh-tests: # Code from module thread: # Code from module thread-tests: # Code from module threadlib: # Code from module time: # Code from module time-tests: # Code from module unistd: # Code from module unistd-tests: # Code from module unsetenv: # Code from module unsetenv-tests: # Code from module vasnprintf: # Code from module vasnprintf-tests: # Code from module verify: # Code from module verify-tests: # Code from module vsnprintf: # Code from module vsnprintf-tests: # Code from module wchar: # Code from module wchar-tests: # Code from module wcrtomb: # Code from module wcrtomb-tests: # Code from module wctob: # Code from module wctomb: # Code from module wctype-h: # Code from module wctype-h-tests: # Code from module xsize: # Code from module yield: if test -n "$ac_tool_prefix"; then for ac_prog in ar lib "link -lib" do # Extract the first word of "$ac_tool_prefix$ac_prog", so it can be a program name with args. set dummy $ac_tool_prefix$ac_prog; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... 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" >&6; } if ${lt_cv_nm_interface+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_nm_interface="BSD nm" echo "int some_variable = 0;" > conftest.$ac_ext (eval echo "\"\$as_me:$LINENO: $ac_compile\"" >&5) (eval "$ac_compile" 2>conftest.err) cat conftest.err >&5 (eval echo "\"\$as_me:$LINENO: $NM \\\"conftest.$ac_objext\\\"\"" >&5) (eval "$NM \"conftest.$ac_objext\"" 2>conftest.err > conftest.out) cat conftest.err >&5 (eval echo "\"\$as_me:$LINENO: output\"" >&5) cat conftest.out >&5 if $GREP 'External.*some_variable' conftest.out > /dev/null; then lt_cv_nm_interface="MS dumpbin" fi rm -f conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_nm_interface" >&5 $as_echo "$lt_cv_nm_interface" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether ln -s works" >&5 $as_echo_n "checking whether ln -s works... " >&6; } LN_S=$as_ln_s if test "$LN_S" = "ln -s"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: yes" >&5 $as_echo "yes" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no, using $LN_S" >&5 $as_echo "no, using $LN_S" >&6; } fi # find the maximum length of command line arguments { $as_echo "$as_me:${as_lineno-$LINENO}: checking the maximum length of command line arguments" >&5 $as_echo_n "checking the maximum length of command line arguments... " >&6; } if ${lt_cv_sys_max_cmd_len+:} false; then : $as_echo_n "(cached) " >&6 else i=0 teststring=ABCD case $build_os in msdosdjgpp*) # On DJGPP, this test can blow up pretty badly due to problems in libc # (any single argument exceeding 2000 bytes causes a buffer overrun # during glob expansion). Even if it were fixed, the result of this # check would be larger than it should be. lt_cv_sys_max_cmd_len=12288; # 12K is about right ;; gnu*) # Under GNU Hurd, this test is not required because there is # no limit to the length of command line arguments. # Libtool will interpret -1 as no limit whatsoever lt_cv_sys_max_cmd_len=-1; ;; cygwin* | mingw* | cegcc*) # On Win9x/ME, this test blows up -- it succeeds, but takes # about 5 minutes as the teststring grows exponentially. # Worse, since 9x/ME are not pre-emptively multitasking, # you end up with a "frozen" computer, even though with patience # the test eventually succeeds (with a max line length of 256k). # Instead, let's just punt: use the minimum linelength reported by # all of the supported platforms: 8192 (on NT/2K/XP). lt_cv_sys_max_cmd_len=8192; ;; mint*) # On MiNT this can take a long time and run out of memory. lt_cv_sys_max_cmd_len=8192; ;; amigaos*) # On AmigaOS with pdksh, this test takes hours, literally. # So we just punt and use a minimum line length of 8192. lt_cv_sys_max_cmd_len=8192; ;; bitrig* | darwin* | dragonfly* | freebsd* | netbsd* | openbsd*) # This has been around since 386BSD, at least. Likely further. if test -x /sbin/sysctl; then lt_cv_sys_max_cmd_len=`/sbin/sysctl -n kern.argmax` elif test -x /usr/sbin/sysctl; then lt_cv_sys_max_cmd_len=`/usr/sbin/sysctl -n kern.argmax` else lt_cv_sys_max_cmd_len=65536 # usable default for all BSDs fi # And add a safety zone lt_cv_sys_max_cmd_len=`expr $lt_cv_sys_max_cmd_len \/ 4` lt_cv_sys_max_cmd_len=`expr $lt_cv_sys_max_cmd_len \* 3` ;; interix*) # We know the value 262144 and hardcode it with a safety zone (like BSD) lt_cv_sys_max_cmd_len=196608 ;; os2*) # The test takes a long time on OS/2. lt_cv_sys_max_cmd_len=8192 ;; osf*) # Dr. Hans Ekkehard Plesser reports seeing a kernel panic running configure # due to this test when exec_disable_arg_limit is 1 on Tru64. It is not # nice to cause kernel panics so lets avoid the loop below. # First set a reasonable default. lt_cv_sys_max_cmd_len=16384 # if test -x /sbin/sysconfig; then case `/sbin/sysconfig -q proc exec_disable_arg_limit` in *1*) lt_cv_sys_max_cmd_len=-1 ;; esac fi ;; sco3.2v5*) lt_cv_sys_max_cmd_len=102400 ;; sysv5* | sco5v6* | sysv4.2uw2*) kargmax=`grep ARG_MAX /etc/conf/cf.d/stune 2>/dev/null` if test -n "$kargmax"; then lt_cv_sys_max_cmd_len=`echo $kargmax | sed 's/.*[ ]//'` else lt_cv_sys_max_cmd_len=32768 fi ;; *) lt_cv_sys_max_cmd_len=`(getconf ARG_MAX) 2> /dev/null` if test -n "$lt_cv_sys_max_cmd_len" && \ test undefined != "$lt_cv_sys_max_cmd_len"; then lt_cv_sys_max_cmd_len=`expr $lt_cv_sys_max_cmd_len \/ 4` lt_cv_sys_max_cmd_len=`expr $lt_cv_sys_max_cmd_len \* 3` else # Make teststring a little bigger before we do anything with it. # a 1K string should be a reasonable start. for i in 1 2 3 4 5 6 7 8; do teststring=$teststring$teststring done SHELL=${SHELL-${CONFIG_SHELL-/bin/sh}} # If test is not a shell built-in, we'll probably end up computing a # maximum length that is only half of the actual maximum length, but # we can't tell. while { test X`env echo "$teststring$teststring" 2>/dev/null` \ = "X$teststring$teststring"; } >/dev/null 2>&1 && test 17 != "$i" # 1/2 MB should be enough do i=`expr $i + 1` teststring=$teststring$teststring done # Only check the string length outside the loop. lt_cv_sys_max_cmd_len=`expr "X$teststring" : ".*" 2>&1` teststring= # Add a significant safety factor because C++ compilers can tack on # massive amounts of additional arguments before passing them to the # linker. It appears as though 1/2 is a usable value. lt_cv_sys_max_cmd_len=`expr $lt_cv_sys_max_cmd_len \/ 2` fi ;; esac fi if test -n "$lt_cv_sys_max_cmd_len"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_sys_max_cmd_len" >&5 $as_echo "$lt_cv_sys_max_cmd_len" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: none" >&5 $as_echo "none" >&6; } fi max_cmd_len=$lt_cv_sys_max_cmd_len : ${CP="cp -f"} : ${MV="mv -f"} : ${RM="rm -f"} if ( (MAIL=60; unset MAIL) || exit) >/dev/null 2>&1; then lt_unset=unset else lt_unset=false fi # test EBCDIC or ASCII case `echo X|tr X '\101'` in A) # ASCII based system # \n is not interpreted correctly by Solaris 8 /usr/ucb/tr lt_SP2NL='tr \040 \012' lt_NL2SP='tr \015\012 \040\040' ;; *) # EBCDIC based system lt_SP2NL='tr \100 \n' lt_NL2SP='tr \r\n \100\100' ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking how to convert $build file names to $host format" >&5 $as_echo_n "checking how to convert $build file names to $host format... " >&6; } if ${lt_cv_to_host_file_cmd+:} false; then : $as_echo_n "(cached) " >&6 else case $host in *-*-mingw* ) case $build in *-*-mingw* ) # actually msys lt_cv_to_host_file_cmd=func_convert_file_msys_to_w32 ;; *-*-cygwin* ) lt_cv_to_host_file_cmd=func_convert_file_cygwin_to_w32 ;; * ) # otherwise, assume *nix lt_cv_to_host_file_cmd=func_convert_file_nix_to_w32 ;; esac ;; *-*-cygwin* ) case $build in *-*-mingw* ) # actually msys lt_cv_to_host_file_cmd=func_convert_file_msys_to_cygwin ;; *-*-cygwin* ) lt_cv_to_host_file_cmd=func_convert_file_noop ;; * ) # otherwise, assume *nix lt_cv_to_host_file_cmd=func_convert_file_nix_to_cygwin ;; esac ;; * ) # unhandled hosts (and "normal" native builds) lt_cv_to_host_file_cmd=func_convert_file_noop ;; esac fi to_host_file_cmd=$lt_cv_to_host_file_cmd { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_to_host_file_cmd" >&5 $as_echo "$lt_cv_to_host_file_cmd" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking how to convert $build file names to toolchain format" >&5 $as_echo_n "checking how to convert $build file names to toolchain format... " >&6; } if ${lt_cv_to_tool_file_cmd+:} false; then : $as_echo_n "(cached) " >&6 else #assume ordinary cross tools, or native build. lt_cv_to_tool_file_cmd=func_convert_file_noop case $host in *-*-mingw* ) case $build in *-*-mingw* ) # actually msys lt_cv_to_tool_file_cmd=func_convert_file_msys_to_w32 ;; esac ;; esac fi to_tool_file_cmd=$lt_cv_to_tool_file_cmd { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_to_tool_file_cmd" >&5 $as_echo "$lt_cv_to_tool_file_cmd" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $LD option to reload object files" >&5 $as_echo_n "checking for $LD option to reload object files... " >&6; } if ${lt_cv_ld_reload_flag+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_ld_reload_flag='-r' fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_ld_reload_flag" >&5 $as_echo "$lt_cv_ld_reload_flag" >&6; } reload_flag=$lt_cv_ld_reload_flag case $reload_flag in "" | " "*) ;; *) reload_flag=" $reload_flag" ;; esac reload_cmds='$LD$reload_flag -o $output$reload_objs' case $host_os in cygwin* | mingw* | pw32* | cegcc*) if test yes != "$GCC"; then reload_cmds=false fi ;; darwin*) if test yes = "$GCC"; then reload_cmds='$LTCC $LTCFLAGS -nostdlib $wl-r -o $output$reload_objs' else reload_cmds='$LD$reload_flag -o $output$reload_objs' fi ;; esac if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}objdump", so it can be a program name with args. set dummy ${ac_tool_prefix}objdump; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_OBJDUMP+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$OBJDUMP"; then ac_cv_prog_OBJDUMP="$OBJDUMP" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_OBJDUMP="${ac_tool_prefix}objdump" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi OBJDUMP=$ac_cv_prog_OBJDUMP if test -n "$OBJDUMP"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $OBJDUMP" >&5 $as_echo "$OBJDUMP" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_OBJDUMP"; then ac_ct_OBJDUMP=$OBJDUMP # Extract the first word of "objdump", so it can be a program name with args. set dummy objdump; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_OBJDUMP+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_OBJDUMP"; then ac_cv_prog_ac_ct_OBJDUMP="$ac_ct_OBJDUMP" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_OBJDUMP="objdump" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_OBJDUMP=$ac_cv_prog_ac_ct_OBJDUMP if test -n "$ac_ct_OBJDUMP"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_OBJDUMP" >&5 $as_echo "$ac_ct_OBJDUMP" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_OBJDUMP" = x; then OBJDUMP="false" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac OBJDUMP=$ac_ct_OBJDUMP fi else OBJDUMP="$ac_cv_prog_OBJDUMP" fi test -z "$OBJDUMP" && OBJDUMP=objdump { $as_echo "$as_me:${as_lineno-$LINENO}: checking how to recognize dependent libraries" >&5 $as_echo_n "checking how to recognize dependent libraries... " >&6; } if ${lt_cv_deplibs_check_method+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_file_magic_cmd='$MAGIC_CMD' lt_cv_file_magic_test_file= lt_cv_deplibs_check_method='unknown' # Need to set the preceding variable on all platforms that support # interlibrary dependencies. # 'none' -- dependencies not supported. # 'unknown' -- same as none, but documents that we really don't know. # 'pass_all' -- all dependencies passed with no checks. # 'test_compile' -- check by making test program. # 'file_magic [[regex]]' -- check by looking for files in library path # that responds to the $file_magic_cmd with a given extended regex. # If you have 'file' or equivalent on your system and you're not sure # whether 'pass_all' will *always* work, you probably want this one. case $host_os in aix[4-9]*) lt_cv_deplibs_check_method=pass_all ;; beos*) lt_cv_deplibs_check_method=pass_all ;; bsdi[45]*) lt_cv_deplibs_check_method='file_magic ELF [0-9][0-9]*-bit [ML]SB (shared object|dynamic lib)' lt_cv_file_magic_cmd='/usr/bin/file -L' lt_cv_file_magic_test_file=/shlib/libc.so ;; cygwin*) # func_win32_libid is a shell function defined in ltmain.sh lt_cv_deplibs_check_method='file_magic ^x86 archive import|^x86 DLL' lt_cv_file_magic_cmd='func_win32_libid' ;; mingw* | pw32*) # Base MSYS/MinGW do not provide the 'file' command needed by # func_win32_libid shell function, so use a weaker test based on 'objdump', # unless we find 'file', for example because we are cross-compiling. if ( file / ) >/dev/null 2>&1; then lt_cv_deplibs_check_method='file_magic ^x86 archive import|^x86 DLL' lt_cv_file_magic_cmd='func_win32_libid' else # Keep this pattern in sync with the one in func_win32_libid. lt_cv_deplibs_check_method='file_magic file format (pei*-i386(.*architecture: i386)?|pe-arm-wince|pe-x86-64)' lt_cv_file_magic_cmd='$OBJDUMP -f' fi ;; cegcc*) # use the weaker test based on 'objdump'. See mingw*. lt_cv_deplibs_check_method='file_magic file format pe-arm-.*little(.*architecture: arm)?' lt_cv_file_magic_cmd='$OBJDUMP -f' ;; darwin* | rhapsody*) lt_cv_deplibs_check_method=pass_all ;; freebsd* | dragonfly*) if echo __ELF__ | $CC -E - | $GREP __ELF__ > /dev/null; then case $host_cpu in i*86 ) # Not sure whether the presence of OpenBSD here was a mistake. # Let's accept both of them until this is cleared up. lt_cv_deplibs_check_method='file_magic (FreeBSD|OpenBSD|DragonFly)/i[3-9]86 (compact )?demand paged shared library' lt_cv_file_magic_cmd=/usr/bin/file lt_cv_file_magic_test_file=`echo /usr/lib/libc.so.*` ;; esac else lt_cv_deplibs_check_method=pass_all fi ;; haiku*) lt_cv_deplibs_check_method=pass_all ;; hpux10.20* | hpux11*) lt_cv_file_magic_cmd=/usr/bin/file case $host_cpu in ia64*) lt_cv_deplibs_check_method='file_magic (s[0-9][0-9][0-9]|ELF-[0-9][0-9]) shared object file - IA64' lt_cv_file_magic_test_file=/usr/lib/hpux32/libc.so ;; hppa*64*) lt_cv_deplibs_check_method='file_magic (s[0-9][0-9][0-9]|ELF[ -][0-9][0-9])(-bit)?( [LM]SB)? shared object( file)?[, -]* PA-RISC [0-9]\.[0-9]' lt_cv_file_magic_test_file=/usr/lib/pa20_64/libc.sl ;; *) lt_cv_deplibs_check_method='file_magic (s[0-9][0-9][0-9]|PA-RISC[0-9]\.[0-9]) shared library' lt_cv_file_magic_test_file=/usr/lib/libc.sl ;; esac ;; interix[3-9]*) # PIC code is broken on Interix 3.x, that's why |\.a not |_pic\.a here lt_cv_deplibs_check_method='match_pattern /lib[^/]+(\.so|\.a)$' ;; irix5* | irix6* | nonstopux*) case $LD in *-32|*"-32 ") libmagic=32-bit;; *-n32|*"-n32 ") libmagic=N32;; *-64|*"-64 ") libmagic=64-bit;; *) libmagic=never-match;; esac lt_cv_deplibs_check_method=pass_all ;; # This must be glibc/ELF. linux* | k*bsd*-gnu | kopensolaris*-gnu | gnu*) lt_cv_deplibs_check_method=pass_all ;; netbsd*) if echo __ELF__ | $CC -E - | $GREP __ELF__ > /dev/null; then lt_cv_deplibs_check_method='match_pattern /lib[^/]+(\.so\.[0-9]+\.[0-9]+|_pic\.a)$' else lt_cv_deplibs_check_method='match_pattern /lib[^/]+(\.so|_pic\.a)$' fi ;; newos6*) lt_cv_deplibs_check_method='file_magic ELF [0-9][0-9]*-bit [ML]SB (executable|dynamic lib)' lt_cv_file_magic_cmd=/usr/bin/file lt_cv_file_magic_test_file=/usr/lib/libnls.so ;; *nto* | *qnx*) lt_cv_deplibs_check_method=pass_all ;; openbsd* | bitrig*) if test -z "`echo __ELF__ | $CC -E - | $GREP __ELF__`"; then lt_cv_deplibs_check_method='match_pattern /lib[^/]+(\.so\.[0-9]+\.[0-9]+|\.so|_pic\.a)$' else lt_cv_deplibs_check_method='match_pattern /lib[^/]+(\.so\.[0-9]+\.[0-9]+|_pic\.a)$' fi ;; osf3* | osf4* | osf5*) lt_cv_deplibs_check_method=pass_all ;; rdos*) lt_cv_deplibs_check_method=pass_all ;; solaris*) lt_cv_deplibs_check_method=pass_all ;; sysv5* | sco3.2v5* | sco5v6* | unixware* | OpenUNIX* | sysv4*uw2*) lt_cv_deplibs_check_method=pass_all ;; sysv4 | sysv4.3*) case $host_vendor in motorola) lt_cv_deplibs_check_method='file_magic ELF [0-9][0-9]*-bit [ML]SB (shared object|dynamic lib) M[0-9][0-9]* Version [0-9]' lt_cv_file_magic_test_file=`echo /usr/lib/libc.so*` ;; ncr) lt_cv_deplibs_check_method=pass_all ;; sequent) lt_cv_file_magic_cmd='/bin/file' lt_cv_deplibs_check_method='file_magic ELF [0-9][0-9]*-bit [LM]SB (shared object|dynamic lib )' ;; sni) lt_cv_file_magic_cmd='/bin/file' lt_cv_deplibs_check_method="file_magic ELF [0-9][0-9]*-bit [LM]SB dynamic lib" lt_cv_file_magic_test_file=/lib/libc.so ;; siemens) lt_cv_deplibs_check_method=pass_all ;; pc) lt_cv_deplibs_check_method=pass_all ;; esac ;; tpf*) lt_cv_deplibs_check_method=pass_all ;; os2*) lt_cv_deplibs_check_method=pass_all ;; esac fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_deplibs_check_method" >&5 $as_echo "$lt_cv_deplibs_check_method" >&6; } file_magic_glob= want_nocaseglob=no if test "$build" = "$host"; then case $host_os in mingw* | pw32*) if ( shopt | grep nocaseglob ) >/dev/null 2>&1; then want_nocaseglob=yes else file_magic_glob=`echo aAbBcCdDeEfFgGhHiIjJkKlLmMnNoOpPqQrRsStTuUvVwWxXyYzZ | $SED -e "s/\(..\)/s\/[\1]\/[\1]\/g;/g"` fi ;; esac fi file_magic_cmd=$lt_cv_file_magic_cmd deplibs_check_method=$lt_cv_deplibs_check_method test -z "$deplibs_check_method" && deplibs_check_method=unknown if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}dlltool", so it can be a program name with args. set dummy ${ac_tool_prefix}dlltool; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_DLLTOOL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$DLLTOOL"; then ac_cv_prog_DLLTOOL="$DLLTOOL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_DLLTOOL="${ac_tool_prefix}dlltool" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi DLLTOOL=$ac_cv_prog_DLLTOOL if test -n "$DLLTOOL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $DLLTOOL" >&5 $as_echo "$DLLTOOL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_DLLTOOL"; then ac_ct_DLLTOOL=$DLLTOOL # Extract the first word of "dlltool", so it can be a program name with args. set dummy dlltool; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_DLLTOOL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_DLLTOOL"; then ac_cv_prog_ac_ct_DLLTOOL="$ac_ct_DLLTOOL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_DLLTOOL="dlltool" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_DLLTOOL=$ac_cv_prog_ac_ct_DLLTOOL if test -n "$ac_ct_DLLTOOL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_DLLTOOL" >&5 $as_echo "$ac_ct_DLLTOOL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_DLLTOOL" = x; then DLLTOOL="false" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac DLLTOOL=$ac_ct_DLLTOOL fi else DLLTOOL="$ac_cv_prog_DLLTOOL" fi test -z "$DLLTOOL" && DLLTOOL=dlltool { $as_echo "$as_me:${as_lineno-$LINENO}: checking how to associate runtime and link libraries" >&5 $as_echo_n "checking how to associate runtime and link libraries... " >&6; } if ${lt_cv_sharedlib_from_linklib_cmd+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_sharedlib_from_linklib_cmd='unknown' case $host_os in cygwin* | mingw* | pw32* | cegcc*) # two different shell functions defined in ltmain.sh; # decide which one to use based on capabilities of $DLLTOOL case `$DLLTOOL --help 2>&1` in *--identify-strict*) lt_cv_sharedlib_from_linklib_cmd=func_cygming_dll_for_implib ;; *) lt_cv_sharedlib_from_linklib_cmd=func_cygming_dll_for_implib_fallback ;; esac ;; *) # fallback: assume linklib IS sharedlib lt_cv_sharedlib_from_linklib_cmd=$ECHO ;; esac fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_sharedlib_from_linklib_cmd" >&5 $as_echo "$lt_cv_sharedlib_from_linklib_cmd" >&6; } sharedlib_from_linklib_cmd=$lt_cv_sharedlib_from_linklib_cmd test -z "$sharedlib_from_linklib_cmd" && sharedlib_from_linklib_cmd=$ECHO if test -n "$ac_tool_prefix"; then for ac_prog in ar do # Extract the first word of "$ac_tool_prefix$ac_prog", so it can be a program name with args. set dummy $ac_tool_prefix$ac_prog; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_AR+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$AR"; then ac_cv_prog_AR="$AR" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_AR="$ac_tool_prefix$ac_prog" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi AR=$ac_cv_prog_AR if test -n "$AR"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $AR" >&5 $as_echo "$AR" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi test -n "$AR" && break done fi if test -z "$AR"; then ac_ct_AR=$AR for ac_prog in ar do # Extract the first word of "$ac_prog", so it can be a program name with args. set dummy $ac_prog; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_AR+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_AR"; then ac_cv_prog_ac_ct_AR="$ac_ct_AR" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_AR="$ac_prog" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_AR=$ac_cv_prog_ac_ct_AR if test -n "$ac_ct_AR"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_AR" >&5 $as_echo "$ac_ct_AR" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi test -n "$ac_ct_AR" && break done if test "x$ac_ct_AR" = x; then AR="false" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac AR=$ac_ct_AR fi fi : ${AR=ar} : ${AR_FLAGS=cru} { $as_echo "$as_me:${as_lineno-$LINENO}: checking for archiver @FILE support" >&5 $as_echo_n "checking for archiver @FILE support... " >&6; } if ${lt_cv_ar_at_file+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_ar_at_file=no cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : echo conftest.$ac_objext > conftest.lst lt_ar_try='$AR $AR_FLAGS libconftest.a @conftest.lst >&5' { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$lt_ar_try\""; } >&5 (eval $lt_ar_try) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } if test 0 -eq "$ac_status"; then # Ensure the archiver fails upon bogus file names. rm -f conftest.$ac_objext libconftest.a { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$lt_ar_try\""; } >&5 (eval $lt_ar_try) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } if test 0 -ne "$ac_status"; then lt_cv_ar_at_file=@ fi fi rm -f conftest.* libconftest.a fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_ar_at_file" >&5 $as_echo "$lt_cv_ar_at_file" >&6; } if test no = "$lt_cv_ar_at_file"; then archiver_list_spec= else archiver_list_spec=$lt_cv_ar_at_file fi if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}strip", so it can be a program name with args. set dummy ${ac_tool_prefix}strip; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_STRIP+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$STRIP"; then ac_cv_prog_STRIP="$STRIP" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_STRIP="${ac_tool_prefix}strip" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi STRIP=$ac_cv_prog_STRIP if test -n "$STRIP"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $STRIP" >&5 $as_echo "$STRIP" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_STRIP"; then ac_ct_STRIP=$STRIP # Extract the first word of "strip", so it can be a program name with args. set dummy strip; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_STRIP+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_STRIP"; then ac_cv_prog_ac_ct_STRIP="$ac_ct_STRIP" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_STRIP="strip" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_STRIP=$ac_cv_prog_ac_ct_STRIP if test -n "$ac_ct_STRIP"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_STRIP" >&5 $as_echo "$ac_ct_STRIP" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_STRIP" = x; then STRIP=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac STRIP=$ac_ct_STRIP fi else STRIP="$ac_cv_prog_STRIP" fi test -z "$STRIP" && STRIP=: if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}ranlib", so it can be a program name with args. set dummy ${ac_tool_prefix}ranlib; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_RANLIB+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$RANLIB"; then ac_cv_prog_RANLIB="$RANLIB" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_RANLIB="${ac_tool_prefix}ranlib" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi RANLIB=$ac_cv_prog_RANLIB if test -n "$RANLIB"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $RANLIB" >&5 $as_echo "$RANLIB" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_RANLIB"; then ac_ct_RANLIB=$RANLIB # Extract the first word of "ranlib", so it can be a program name with args. set dummy ranlib; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_RANLIB+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_RANLIB"; then ac_cv_prog_ac_ct_RANLIB="$ac_ct_RANLIB" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_RANLIB="ranlib" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_RANLIB=$ac_cv_prog_ac_ct_RANLIB if test -n "$ac_ct_RANLIB"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_RANLIB" >&5 $as_echo "$ac_ct_RANLIB" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_RANLIB" = x; then RANLIB=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac RANLIB=$ac_ct_RANLIB fi else RANLIB="$ac_cv_prog_RANLIB" fi test -z "$RANLIB" && RANLIB=: # Determine commands to create old-style static archives. old_archive_cmds='$AR $AR_FLAGS $oldlib$oldobjs' old_postinstall_cmds='chmod 644 $oldlib' old_postuninstall_cmds= if test -n "$RANLIB"; then case $host_os in bitrig* | openbsd*) old_postinstall_cmds="$old_postinstall_cmds~\$RANLIB -t \$tool_oldlib" ;; *) old_postinstall_cmds="$old_postinstall_cmds~\$RANLIB \$tool_oldlib" ;; esac old_archive_cmds="$old_archive_cmds~\$RANLIB \$tool_oldlib" fi case $host_os in darwin*) lock_old_archive_extraction=yes ;; *) lock_old_archive_extraction=no ;; esac # If no C compiler was specified, use CC. LTCC=${LTCC-"$CC"} # If no C compiler flags were specified, use CFLAGS. LTCFLAGS=${LTCFLAGS-"$CFLAGS"} # Allow CC to be a program name with arguments. compiler=$CC # Check for command to grab the raw symbol name followed by C symbol from nm. { $as_echo "$as_me:${as_lineno-$LINENO}: checking command to parse $NM output from $compiler object" >&5 $as_echo_n "checking command to parse $NM output from $compiler object... " >&6; } if ${lt_cv_sys_global_symbol_pipe+:} false; then : $as_echo_n "(cached) " >&6 else # These are sane defaults that work on at least a few old systems. # [They come from Ultrix. What could be older than Ultrix?!! ;)] # Character class describing NM global symbol codes. symcode='[BCDEGRST]' # Regexp to match symbols that can be accessed directly from C. sympat='\([_A-Za-z][_A-Za-z0-9]*\)' # Define system-specific variables. case $host_os in aix*) symcode='[BCDT]' ;; cygwin* | mingw* | pw32* | cegcc*) symcode='[ABCDGISTW]' ;; hpux*) if test ia64 = "$host_cpu"; then symcode='[ABCDEGRST]' fi ;; irix* | nonstopux*) symcode='[BCDEGRST]' ;; osf*) symcode='[BCDEGQRST]' ;; solaris*) symcode='[BDRT]' ;; sco3.2v5*) symcode='[DT]' ;; sysv4.2uw2*) symcode='[DT]' ;; sysv5* | sco5v6* | unixware* | OpenUNIX*) symcode='[ABDT]' ;; sysv4) symcode='[DFNSTU]' ;; esac # If we're using GNU nm, then use its standard symbol codes. case `$NM -V 2>&1` in *GNU* | *'with BFD'*) symcode='[ABCDGIRSTW]' ;; esac if test "$lt_cv_nm_interface" = "MS dumpbin"; then # Gets list of data symbols to import. lt_cv_sys_global_symbol_to_import="sed -n -e 's/^I .* \(.*\)$/\1/p'" # Adjust the below global symbol transforms to fixup imported variables. lt_cdecl_hook=" -e 's/^I .* \(.*\)$/extern __declspec(dllimport) char \1;/p'" lt_c_name_hook=" -e 's/^I .* \(.*\)$/ {\"\1\", (void *) 0},/p'" lt_c_name_lib_hook="\ -e 's/^I .* \(lib.*\)$/ {\"\1\", (void *) 0},/p'\ -e 's/^I .* \(.*\)$/ {\"lib\1\", (void *) 0},/p'" else # Disable hooks by default. lt_cv_sys_global_symbol_to_import= lt_cdecl_hook= lt_c_name_hook= lt_c_name_lib_hook= fi # Transform an extracted symbol line into a proper C declaration. # Some systems (esp. on ia64) link data and code symbols differently, # so use this general approach. lt_cv_sys_global_symbol_to_cdecl="sed -n"\ $lt_cdecl_hook\ " -e 's/^T .* \(.*\)$/extern int \1();/p'"\ " -e 's/^$symcode$symcode* .* \(.*\)$/extern char \1;/p'" # Transform an extracted symbol line into symbol name and symbol address lt_cv_sys_global_symbol_to_c_name_address="sed -n"\ $lt_c_name_hook\ " -e 's/^: \(.*\) .*$/ {\"\1\", (void *) 0},/p'"\ " -e 's/^$symcode$symcode* .* \(.*\)$/ {\"\1\", (void *) \&\1},/p'" # Transform an extracted symbol line into symbol name with lib prefix and # symbol address. lt_cv_sys_global_symbol_to_c_name_address_lib_prefix="sed -n"\ $lt_c_name_lib_hook\ " -e 's/^: \(.*\) .*$/ {\"\1\", (void *) 0},/p'"\ " -e 's/^$symcode$symcode* .* \(lib.*\)$/ {\"\1\", (void *) \&\1},/p'"\ " -e 's/^$symcode$symcode* .* \(.*\)$/ {\"lib\1\", (void *) \&\1},/p'" # Handle CRLF in mingw tool chain opt_cr= case $build_os in mingw*) opt_cr=`$ECHO 'x\{0,1\}' | tr x '\015'` # option cr in regexp ;; esac # Try without a prefix underscore, then with it. for ac_symprfx in "" "_"; do # Transform symcode, sympat, and symprfx into a raw symbol and a C symbol. symxfrm="\\1 $ac_symprfx\\2 \\2" # Write the raw and C identifiers. if test "$lt_cv_nm_interface" = "MS dumpbin"; then # Fake it for dumpbin and say T for any non-static function, # D for any global variable and I for any imported variable. # Also find C++ and __fastcall symbols from MSVC++, # which start with @ or ?. lt_cv_sys_global_symbol_pipe="$AWK '"\ " {last_section=section; section=\$ 3};"\ " /^COFF SYMBOL TABLE/{for(i in hide) delete hide[i]};"\ " /Section length .*#relocs.*(pick any)/{hide[last_section]=1};"\ " /^ *Symbol name *: /{split(\$ 0,sn,\":\"); si=substr(sn[2],2)};"\ " /^ *Type *: code/{print \"T\",si,substr(si,length(prfx))};"\ " /^ *Type *: data/{print \"I\",si,substr(si,length(prfx))};"\ " \$ 0!~/External *\|/{next};"\ " / 0+ UNDEF /{next}; / UNDEF \([^|]\)*()/{next};"\ " {if(hide[section]) next};"\ " {f=\"D\"}; \$ 0~/\(\).*\|/{f=\"T\"};"\ " {split(\$ 0,a,/\||\r/); split(a[2],s)};"\ " s[1]~/^[@?]/{print f,s[1],s[1]; next};"\ " s[1]~prfx {split(s[1],t,\"@\"); print f,t[1],substr(t[1],length(prfx))}"\ " ' prfx=^$ac_symprfx" else lt_cv_sys_global_symbol_pipe="sed -n -e 's/^.*[ ]\($symcode$symcode*\)[ ][ ]*$ac_symprfx$sympat$opt_cr$/$symxfrm/p'" fi lt_cv_sys_global_symbol_pipe="$lt_cv_sys_global_symbol_pipe | sed '/ __gnu_lto/d'" # Check to see that the pipe works correctly. pipe_works=no rm -f conftest* cat > conftest.$ac_ext <<_LT_EOF #ifdef __cplusplus extern "C" { #endif char nm_test_var; void nm_test_func(void); void nm_test_func(void){} #ifdef __cplusplus } #endif int main(){nm_test_var='a';nm_test_func();return(0);} _LT_EOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_compile\""; } >&5 (eval $ac_compile) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; }; then # Now try to grab the symbols. nlist=conftest.nm if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$NM conftest.$ac_objext \| "$lt_cv_sys_global_symbol_pipe" \> $nlist\""; } >&5 (eval $NM conftest.$ac_objext \| "$lt_cv_sys_global_symbol_pipe" \> $nlist) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s "$nlist"; then # Try sorting and uniquifying the output. if sort "$nlist" | uniq > "$nlist"T; then mv -f "$nlist"T "$nlist" else rm -f "$nlist"T fi # Make sure that we snagged all the symbols we need. if $GREP ' nm_test_var$' "$nlist" >/dev/null; then if $GREP ' nm_test_func$' "$nlist" >/dev/null; then cat <<_LT_EOF > conftest.$ac_ext /* Keep this code in sync between libtool.m4, ltmain, lt_system.h, and tests. */ #if defined _WIN32 || defined __CYGWIN__ || defined _WIN32_WCE /* DATA imports from DLLs on WIN32 can't be const, because runtime relocations are performed -- see ld's documentation on pseudo-relocs. */ # define LT_DLSYM_CONST #elif defined __osf__ /* This system does not cope well with relocations in const data. */ # define LT_DLSYM_CONST #else # define LT_DLSYM_CONST const #endif #ifdef __cplusplus extern "C" { #endif _LT_EOF # Now generate the symbol file. eval "$lt_cv_sys_global_symbol_to_cdecl"' < "$nlist" | $GREP -v main >> conftest.$ac_ext' cat <<_LT_EOF >> conftest.$ac_ext /* The mapping between symbol names and symbols. */ LT_DLSYM_CONST struct { const char *name; void *address; } lt__PROGRAM__LTX_preloaded_symbols[] = { { "@PROGRAM@", (void *) 0 }, _LT_EOF $SED "s/^$symcode$symcode* .* \(.*\)$/ {\"\1\", (void *) \&\1},/" < "$nlist" | $GREP -v main >> conftest.$ac_ext cat <<\_LT_EOF >> conftest.$ac_ext {0, (void *) 0} }; /* This works around a problem in FreeBSD linker */ #ifdef FREEBSD_WORKAROUND static const void *lt_preloaded_setup() { return lt__PROGRAM__LTX_preloaded_symbols; } #endif #ifdef __cplusplus } #endif _LT_EOF # Now try linking the two files. mv conftest.$ac_objext conftstm.$ac_objext lt_globsym_save_LIBS=$LIBS lt_globsym_save_CFLAGS=$CFLAGS LIBS=conftstm.$ac_objext CFLAGS="$CFLAGS$lt_prog_compiler_no_builtin_flag" if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then pipe_works=yes fi LIBS=$lt_globsym_save_LIBS CFLAGS=$lt_globsym_save_CFLAGS else echo "cannot find nm_test_func in $nlist" >&5 fi else echo "cannot find nm_test_var in $nlist" >&5 fi else echo "cannot run $lt_cv_sys_global_symbol_pipe" >&5 fi else echo "$progname: failed program was:" >&5 cat conftest.$ac_ext >&5 fi rm -rf conftest* conftst* # Do not use the global_symbol_pipe unless it works. if test yes = "$pipe_works"; then break else lt_cv_sys_global_symbol_pipe= fi done fi if test -z "$lt_cv_sys_global_symbol_pipe"; then lt_cv_sys_global_symbol_to_cdecl= fi if test -z "$lt_cv_sys_global_symbol_pipe$lt_cv_sys_global_symbol_to_cdecl"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: failed" >&5 $as_echo "failed" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: ok" >&5 $as_echo "ok" >&6; } fi # Response file support. if test "$lt_cv_nm_interface" = "MS dumpbin"; then nm_file_list_spec='@' elif $NM --help 2>/dev/null | grep '[@]FILE' >/dev/null; then nm_file_list_spec='@' fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for sysroot" >&5 $as_echo_n "checking for sysroot... " >&6; } # Check whether --with-sysroot was given. if test "${with_sysroot+set}" = set; then : withval=$with_sysroot; else with_sysroot=no fi lt_sysroot= case $with_sysroot in #( yes) if test yes = "$GCC"; then lt_sysroot=`$CC --print-sysroot 2>/dev/null` fi ;; #( /*) lt_sysroot=`echo "$with_sysroot" | sed -e "$sed_quote_subst"` ;; #( no|'') ;; #( *) { $as_echo "$as_me:${as_lineno-$LINENO}: result: $with_sysroot" >&5 $as_echo "$with_sysroot" >&6; } as_fn_error $? "The sysroot must be an absolute path." "$LINENO" 5 ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: result: ${lt_sysroot:-no}" >&5 $as_echo "${lt_sysroot:-no}" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a working dd" >&5 $as_echo_n "checking for a working dd... " >&6; } if ${ac_cv_path_lt_DD+:} false; then : $as_echo_n "(cached) " >&6 else printf 0123456789abcdef0123456789abcdef >conftest.i cat conftest.i conftest.i >conftest2.i : ${lt_DD:=$DD} if test -z "$lt_DD"; then ac_path_lt_DD_found=false # Loop through the user's path and test for each of PROGNAME-LIST as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_prog in dd; do for ac_exec_ext in '' $ac_executable_extensions; do ac_path_lt_DD="$as_dir/$ac_prog$ac_exec_ext" as_fn_executable_p "$ac_path_lt_DD" || continue if "$ac_path_lt_DD" bs=32 count=1 conftest.out 2>/dev/null; then cmp -s conftest.i conftest.out \ && ac_cv_path_lt_DD="$ac_path_lt_DD" ac_path_lt_DD_found=: fi $ac_path_lt_DD_found && break 3 done done done IFS=$as_save_IFS if test -z "$ac_cv_path_lt_DD"; then : fi else ac_cv_path_lt_DD=$lt_DD fi rm -f conftest.i conftest2.i conftest.out fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_path_lt_DD" >&5 $as_echo "$ac_cv_path_lt_DD" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking how to truncate binary pipes" >&5 $as_echo_n "checking how to truncate binary pipes... " >&6; } if ${lt_cv_truncate_bin+:} false; then : $as_echo_n "(cached) " >&6 else printf 0123456789abcdef0123456789abcdef >conftest.i cat conftest.i conftest.i >conftest2.i lt_cv_truncate_bin= if "$ac_cv_path_lt_DD" bs=32 count=1 conftest.out 2>/dev/null; then cmp -s conftest.i conftest.out \ && lt_cv_truncate_bin="$ac_cv_path_lt_DD bs=4096 count=1" fi rm -f conftest.i conftest2.i conftest.out test -z "$lt_cv_truncate_bin" && lt_cv_truncate_bin="$SED -e 4q" fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_truncate_bin" >&5 $as_echo "$lt_cv_truncate_bin" >&6; } # Calculate cc_basename. Skip known compiler wrappers and cross-prefix. func_cc_basename () { for cc_temp in $*""; do case $cc_temp in compile | *[\\/]compile | ccache | *[\\/]ccache ) ;; distcc | *[\\/]distcc | purify | *[\\/]purify ) ;; \-*) ;; *) break;; esac done func_cc_basename_result=`$ECHO "$cc_temp" | $SED "s%.*/%%; s%^$host_alias-%%"` } # Check whether --enable-libtool-lock was given. if test "${enable_libtool_lock+set}" = set; then : enableval=$enable_libtool_lock; fi test no = "$enable_libtool_lock" || enable_libtool_lock=yes # Some flags need to be propagated to the compiler or linker for good # libtool support. case $host in ia64-*-hpux*) # Find out what ABI is being produced by ac_compile, and set mode # options accordingly. echo 'int i;' > conftest.$ac_ext if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_compile\""; } >&5 (eval $ac_compile) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; }; then case `/usr/bin/file conftest.$ac_objext` in *ELF-32*) HPUX_IA64_MODE=32 ;; *ELF-64*) HPUX_IA64_MODE=64 ;; esac fi rm -rf conftest* ;; *-*-irix6*) # Find out what ABI is being produced by ac_compile, and set linker # options accordingly. echo '#line '$LINENO' "configure"' > conftest.$ac_ext if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_compile\""; } >&5 (eval $ac_compile) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; }; then if test yes = "$lt_cv_prog_gnu_ld"; then case `/usr/bin/file conftest.$ac_objext` in *32-bit*) LD="${LD-ld} -melf32bsmip" ;; *N32*) LD="${LD-ld} -melf32bmipn32" ;; *64-bit*) LD="${LD-ld} -melf64bmip" ;; esac else case `/usr/bin/file conftest.$ac_objext` in *32-bit*) LD="${LD-ld} -32" ;; *N32*) LD="${LD-ld} -n32" ;; *64-bit*) LD="${LD-ld} -64" ;; esac fi fi rm -rf conftest* ;; mips64*-*linux*) # Find out what ABI is being produced by ac_compile, and set linker # options accordingly. echo '#line '$LINENO' "configure"' > conftest.$ac_ext if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_compile\""; } >&5 (eval $ac_compile) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; }; then emul=elf case `/usr/bin/file conftest.$ac_objext` in *32-bit*) emul="${emul}32" ;; *64-bit*) emul="${emul}64" ;; esac case `/usr/bin/file conftest.$ac_objext` in *MSB*) emul="${emul}btsmip" ;; *LSB*) emul="${emul}ltsmip" ;; esac case `/usr/bin/file conftest.$ac_objext` in *N32*) emul="${emul}n32" ;; esac LD="${LD-ld} -m $emul" fi rm -rf conftest* ;; x86_64-*kfreebsd*-gnu|x86_64-*linux*|powerpc*-*linux*| \ s390*-*linux*|s390*-*tpf*|sparc*-*linux*) # Find out what ABI is being produced by ac_compile, and set linker # options accordingly. Note that the listed cases only cover the # situations where additional linker options are needed (such as when # doing 32-bit compilation for a host where ld defaults to 64-bit, or # vice versa); the common cases where no linker options are needed do # not appear in the list. echo 'int i;' > conftest.$ac_ext if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_compile\""; } >&5 (eval $ac_compile) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; }; then case `/usr/bin/file conftest.o` in *32-bit*) case $host in x86_64-*kfreebsd*-gnu) LD="${LD-ld} -m elf_i386_fbsd" ;; x86_64-*linux*) case `/usr/bin/file conftest.o` in *x86-64*) LD="${LD-ld} -m elf32_x86_64" ;; *) LD="${LD-ld} -m elf_i386" ;; esac ;; powerpc64le-*linux*) LD="${LD-ld} -m elf32lppclinux" ;; powerpc64-*linux*) LD="${LD-ld} -m elf32ppclinux" ;; s390x-*linux*) LD="${LD-ld} -m elf_s390" ;; sparc64-*linux*) LD="${LD-ld} -m elf32_sparc" ;; esac ;; *64-bit*) case $host in x86_64-*kfreebsd*-gnu) LD="${LD-ld} -m elf_x86_64_fbsd" ;; x86_64-*linux*) LD="${LD-ld} -m elf_x86_64" ;; powerpcle-*linux*) LD="${LD-ld} -m elf64lppc" ;; powerpc-*linux*) LD="${LD-ld} -m elf64ppc" ;; s390*-*linux*|s390*-*tpf*) LD="${LD-ld} -m elf64_s390" ;; sparc*-*linux*) LD="${LD-ld} -m elf64_sparc" ;; esac ;; esac fi rm -rf conftest* ;; *-*-sco3.2v5*) # On SCO OpenServer 5, we need -belf to get full-featured binaries. SAVE_CFLAGS=$CFLAGS CFLAGS="$CFLAGS -belf" { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether the C compiler needs -belf" >&5 $as_echo_n "checking whether the C compiler needs -belf... " >&6; } if ${lt_cv_cc_needs_belf+:} false; then : $as_echo_n "(cached) " >&6 else ac_ext=c ac_cpp='$CPP $CPPFLAGS' ac_compile='$CC -c $CFLAGS $CPPFLAGS conftest.$ac_ext >&5' ac_link='$CC -o conftest$ac_exeext $CFLAGS $CPPFLAGS $LDFLAGS conftest.$ac_ext $LIBS >&5' ac_compiler_gnu=$ac_cv_c_compiler_gnu cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ int main () { ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : lt_cv_cc_needs_belf=yes else lt_cv_cc_needs_belf=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext ac_ext=c ac_cpp='$CPP $CPPFLAGS' ac_compile='$CC -c $CFLAGS $CPPFLAGS conftest.$ac_ext >&5' ac_link='$CC -o conftest$ac_exeext $CFLAGS $CPPFLAGS $LDFLAGS conftest.$ac_ext $LIBS >&5' ac_compiler_gnu=$ac_cv_c_compiler_gnu fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_cc_needs_belf" >&5 $as_echo "$lt_cv_cc_needs_belf" >&6; } if test yes != "$lt_cv_cc_needs_belf"; then # this is probably gcc 2.8.0, egcs 1.0 or newer; no need for -belf CFLAGS=$SAVE_CFLAGS fi ;; *-*solaris*) # Find out what ABI is being produced by ac_compile, and set linker # options accordingly. echo 'int i;' > conftest.$ac_ext if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_compile\""; } >&5 (eval $ac_compile) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; }; then case `/usr/bin/file conftest.o` in *64-bit*) case $lt_cv_prog_gnu_ld in yes*) case $host in i?86-*-solaris*|x86_64-*-solaris*) LD="${LD-ld} -m elf_x86_64" ;; sparc*-*-solaris*) LD="${LD-ld} -m elf64_sparc" ;; esac # GNU ld 2.21 introduced _sol2 emulations. Use them if available. if ${LD-ld} -V | grep _sol2 >/dev/null 2>&1; then LD=${LD-ld}_sol2 fi ;; *) if ${LD-ld} -64 -r -o conftest2.o conftest.o >/dev/null 2>&1; then LD="${LD-ld} -64" fi ;; esac ;; esac fi rm -rf conftest* ;; esac need_locks=$enable_libtool_lock if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}mt", so it can be a program name with args. set dummy ${ac_tool_prefix}mt; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_MANIFEST_TOOL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$MANIFEST_TOOL"; then ac_cv_prog_MANIFEST_TOOL="$MANIFEST_TOOL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_MANIFEST_TOOL="${ac_tool_prefix}mt" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi MANIFEST_TOOL=$ac_cv_prog_MANIFEST_TOOL if test -n "$MANIFEST_TOOL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $MANIFEST_TOOL" >&5 $as_echo "$MANIFEST_TOOL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_MANIFEST_TOOL"; then ac_ct_MANIFEST_TOOL=$MANIFEST_TOOL # Extract the first word of "mt", so it can be a program name with args. set dummy mt; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_MANIFEST_TOOL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_MANIFEST_TOOL"; then ac_cv_prog_ac_ct_MANIFEST_TOOL="$ac_ct_MANIFEST_TOOL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_MANIFEST_TOOL="mt" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_MANIFEST_TOOL=$ac_cv_prog_ac_ct_MANIFEST_TOOL if test -n "$ac_ct_MANIFEST_TOOL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_MANIFEST_TOOL" >&5 $as_echo "$ac_ct_MANIFEST_TOOL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_MANIFEST_TOOL" = x; then MANIFEST_TOOL=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac MANIFEST_TOOL=$ac_ct_MANIFEST_TOOL fi else MANIFEST_TOOL="$ac_cv_prog_MANIFEST_TOOL" fi test -z "$MANIFEST_TOOL" && MANIFEST_TOOL=mt { $as_echo "$as_me:${as_lineno-$LINENO}: checking if $MANIFEST_TOOL is a manifest tool" >&5 $as_echo_n "checking if $MANIFEST_TOOL is a manifest tool... " >&6; } if ${lt_cv_path_mainfest_tool+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_path_mainfest_tool=no echo "$as_me:$LINENO: $MANIFEST_TOOL '-?'" >&5 $MANIFEST_TOOL '-?' 2>conftest.err > conftest.out cat conftest.err >&5 if $GREP 'Manifest Tool' conftest.out > /dev/null; then lt_cv_path_mainfest_tool=yes fi rm -f conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_path_mainfest_tool" >&5 $as_echo "$lt_cv_path_mainfest_tool" >&6; } if test yes != "$lt_cv_path_mainfest_tool"; then MANIFEST_TOOL=: fi case $host_os in rhapsody* | darwin*) if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}dsymutil", so it can be a program name with args. set dummy ${ac_tool_prefix}dsymutil; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_DSYMUTIL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$DSYMUTIL"; then ac_cv_prog_DSYMUTIL="$DSYMUTIL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_DSYMUTIL="${ac_tool_prefix}dsymutil" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi DSYMUTIL=$ac_cv_prog_DSYMUTIL if test -n "$DSYMUTIL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $DSYMUTIL" >&5 $as_echo "$DSYMUTIL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_DSYMUTIL"; then ac_ct_DSYMUTIL=$DSYMUTIL # Extract the first word of "dsymutil", so it can be a program name with args. set dummy dsymutil; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_DSYMUTIL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_DSYMUTIL"; then ac_cv_prog_ac_ct_DSYMUTIL="$ac_ct_DSYMUTIL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_DSYMUTIL="dsymutil" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_DSYMUTIL=$ac_cv_prog_ac_ct_DSYMUTIL if test -n "$ac_ct_DSYMUTIL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_DSYMUTIL" >&5 $as_echo "$ac_ct_DSYMUTIL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_DSYMUTIL" = x; then DSYMUTIL=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac DSYMUTIL=$ac_ct_DSYMUTIL fi else DSYMUTIL="$ac_cv_prog_DSYMUTIL" fi if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}nmedit", so it can be a program name with args. set dummy ${ac_tool_prefix}nmedit; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_NMEDIT+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$NMEDIT"; then ac_cv_prog_NMEDIT="$NMEDIT" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_NMEDIT="${ac_tool_prefix}nmedit" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi NMEDIT=$ac_cv_prog_NMEDIT if test -n "$NMEDIT"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $NMEDIT" >&5 $as_echo "$NMEDIT" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_NMEDIT"; then ac_ct_NMEDIT=$NMEDIT # Extract the first word of "nmedit", so it can be a program name with args. set dummy nmedit; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_NMEDIT+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_NMEDIT"; then ac_cv_prog_ac_ct_NMEDIT="$ac_ct_NMEDIT" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_NMEDIT="nmedit" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_NMEDIT=$ac_cv_prog_ac_ct_NMEDIT if test -n "$ac_ct_NMEDIT"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_NMEDIT" >&5 $as_echo "$ac_ct_NMEDIT" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_NMEDIT" = x; then NMEDIT=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac NMEDIT=$ac_ct_NMEDIT fi else NMEDIT="$ac_cv_prog_NMEDIT" fi if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}lipo", so it can be a program name with args. set dummy ${ac_tool_prefix}lipo; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_LIPO+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$LIPO"; then ac_cv_prog_LIPO="$LIPO" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_LIPO="${ac_tool_prefix}lipo" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi LIPO=$ac_cv_prog_LIPO if test -n "$LIPO"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $LIPO" >&5 $as_echo "$LIPO" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_LIPO"; then ac_ct_LIPO=$LIPO # Extract the first word of "lipo", so it can be a program name with args. set dummy lipo; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_LIPO+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_LIPO"; then ac_cv_prog_ac_ct_LIPO="$ac_ct_LIPO" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_LIPO="lipo" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_LIPO=$ac_cv_prog_ac_ct_LIPO if test -n "$ac_ct_LIPO"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_LIPO" >&5 $as_echo "$ac_ct_LIPO" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_LIPO" = x; then LIPO=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac LIPO=$ac_ct_LIPO fi else LIPO="$ac_cv_prog_LIPO" fi if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}otool", so it can be a program name with args. set dummy ${ac_tool_prefix}otool; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_OTOOL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$OTOOL"; then ac_cv_prog_OTOOL="$OTOOL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_OTOOL="${ac_tool_prefix}otool" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi OTOOL=$ac_cv_prog_OTOOL if test -n "$OTOOL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $OTOOL" >&5 $as_echo "$OTOOL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_OTOOL"; then ac_ct_OTOOL=$OTOOL # Extract the first word of "otool", so it can be a program name with args. set dummy otool; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_OTOOL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_OTOOL"; then ac_cv_prog_ac_ct_OTOOL="$ac_ct_OTOOL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_OTOOL="otool" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_OTOOL=$ac_cv_prog_ac_ct_OTOOL if test -n "$ac_ct_OTOOL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_OTOOL" >&5 $as_echo "$ac_ct_OTOOL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_OTOOL" = x; then OTOOL=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac OTOOL=$ac_ct_OTOOL fi else OTOOL="$ac_cv_prog_OTOOL" fi if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}otool64", so it can be a program name with args. set dummy ${ac_tool_prefix}otool64; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_OTOOL64+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$OTOOL64"; then ac_cv_prog_OTOOL64="$OTOOL64" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_OTOOL64="${ac_tool_prefix}otool64" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi OTOOL64=$ac_cv_prog_OTOOL64 if test -n "$OTOOL64"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $OTOOL64" >&5 $as_echo "$OTOOL64" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_OTOOL64"; then ac_ct_OTOOL64=$OTOOL64 # Extract the first word of "otool64", so it can be a program name with args. set dummy otool64; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_OTOOL64+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_OTOOL64"; then ac_cv_prog_ac_ct_OTOOL64="$ac_ct_OTOOL64" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_OTOOL64="otool64" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_OTOOL64=$ac_cv_prog_ac_ct_OTOOL64 if test -n "$ac_ct_OTOOL64"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_OTOOL64" >&5 $as_echo "$ac_ct_OTOOL64" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_OTOOL64" = x; then OTOOL64=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac OTOOL64=$ac_ct_OTOOL64 fi else OTOOL64="$ac_cv_prog_OTOOL64" fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for -single_module linker flag" >&5 $as_echo_n "checking for -single_module linker flag... " >&6; } if ${lt_cv_apple_cc_single_mod+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_apple_cc_single_mod=no if test -z "$LT_MULTI_MODULE"; then # By default we will add the -single_module flag. You can override # by either setting the environment variable LT_MULTI_MODULE # non-empty at configure time, or by adding -multi_module to the # link flags. rm -rf libconftest.dylib* echo "int foo(void){return 1;}" > conftest.c echo "$LTCC $LTCFLAGS $LDFLAGS -o libconftest.dylib \ -dynamiclib -Wl,-single_module conftest.c" >&5 $LTCC $LTCFLAGS $LDFLAGS -o libconftest.dylib \ -dynamiclib -Wl,-single_module conftest.c 2>conftest.err _lt_result=$? # If there is a non-empty error log, and "single_module" # appears in it, assume the flag caused a linker warning if test -s conftest.err && $GREP single_module conftest.err; then cat conftest.err >&5 # Otherwise, if the output was created with a 0 exit code from # the compiler, it worked. elif test -f libconftest.dylib && test 0 = "$_lt_result"; then lt_cv_apple_cc_single_mod=yes else cat conftest.err >&5 fi rm -rf libconftest.dylib* rm -f conftest.* fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_apple_cc_single_mod" >&5 $as_echo "$lt_cv_apple_cc_single_mod" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking for -exported_symbols_list linker flag" >&5 $as_echo_n "checking for -exported_symbols_list linker flag... " >&6; } if ${lt_cv_ld_exported_symbols_list+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_ld_exported_symbols_list=no save_LDFLAGS=$LDFLAGS echo "_main" > conftest.sym LDFLAGS="$LDFLAGS -Wl,-exported_symbols_list,conftest.sym" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ int main () { ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : lt_cv_ld_exported_symbols_list=yes else lt_cv_ld_exported_symbols_list=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LDFLAGS=$save_LDFLAGS fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_ld_exported_symbols_list" >&5 $as_echo "$lt_cv_ld_exported_symbols_list" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking for -force_load linker flag" >&5 $as_echo_n "checking for -force_load linker flag... 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If you *** really care for shared libraries, you may want to install binutils *** 2.20 or above, or modify your PATH so that a non-GNU linker is found. *** You will then need to restart the configuration process. _LT_EOF fi ;; amigaos*) case $host_cpu in powerpc) # see comment about AmigaOS4 .so support archive_cmds='$CC -shared $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' archive_expsym_cmds='' ;; m68k) archive_cmds='$RM $output_objdir/a2ixlibrary.data~$ECHO "#define NAME $libname" > $output_objdir/a2ixlibrary.data~$ECHO "#define LIBRARY_ID 1" >> $output_objdir/a2ixlibrary.data~$ECHO "#define VERSION $major" >> $output_objdir/a2ixlibrary.data~$ECHO "#define REVISION $revision" >> $output_objdir/a2ixlibrary.data~$AR $AR_FLAGS $lib $libobjs~$RANLIB $lib~(cd $output_objdir && a2ixlibrary -32)' hardcode_libdir_flag_spec='-L$libdir' hardcode_minus_L=yes ;; esac ;; beos*) if $LD --help 2>&1 | $GREP ': supported targets:.* elf' > /dev/null; then allow_undefined_flag=unsupported # Joseph Beckenbach says some releases of gcc # support --undefined. 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FIXME archive_cmds='$CC -nostart $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' else ld_shlibs=no fi ;; cygwin* | mingw* | pw32* | cegcc*) # _LT_TAGVAR(hardcode_libdir_flag_spec, ) is actually meaningless, # as there is no search path for DLLs. hardcode_libdir_flag_spec='-L$libdir' export_dynamic_flag_spec='$wl--export-all-symbols' allow_undefined_flag=unsupported always_export_symbols=no enable_shared_with_static_runtimes=yes export_symbols_cmds='$NM $libobjs $convenience | $global_symbol_pipe | $SED -e '\''/^[BCDGRS][ ]/s/.*[ ]\([^ ]*\)/\1 DATA/;s/^.*[ ]__nm__\([^ ]*\)[ ][^ ]*/\1 DATA/;/^I[ ]/d;/^[AITW][ ]/s/.* //'\'' | sort | uniq > $export_symbols' exclude_expsyms='[_]+GLOBAL_OFFSET_TABLE_|[_]+GLOBAL__[FID]_.*|[_]+head_[A-Za-z0-9_]+_dll|[A-Za-z0-9_]+_dll_iname' if $LD --help 2>&1 | $GREP 'auto-import' > /dev/null; then archive_cmds='$CC -shared $libobjs $deplibs $compiler_flags -o $output_objdir/$soname $wl--enable-auto-image-base -Xlinker --out-implib -Xlinker $lib' # If the export-symbols file already is a .def file, use it as # is; otherwise, prepend EXPORTS... archive_expsym_cmds='if test DEF = "`$SED -n -e '\''s/^[ ]*//'\'' -e '\''/^\(;.*\)*$/d'\'' -e '\''s/^\(EXPORTS\|LIBRARY\)\([ ].*\)*$/DEF/p'\'' -e q $export_symbols`" ; then cp $export_symbols $output_objdir/$soname.def; else echo EXPORTS > $output_objdir/$soname.def; cat $export_symbols >> $output_objdir/$soname.def; fi~ $CC -shared $output_objdir/$soname.def $libobjs $deplibs $compiler_flags -o $output_objdir/$soname $wl--enable-auto-image-base -Xlinker --out-implib -Xlinker $lib' else ld_shlibs=no fi ;; haiku*) archive_cmds='$CC -shared $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' link_all_deplibs=yes ;; os2*) hardcode_libdir_flag_spec='-L$libdir' hardcode_minus_L=yes allow_undefined_flag=unsupported shrext_cmds=.dll archive_cmds='$ECHO "LIBRARY ${soname%$shared_ext} INITINSTANCE TERMINSTANCE" > $output_objdir/$libname.def~ $ECHO "DESCRIPTION \"$libname\"" >> $output_objdir/$libname.def~ $ECHO "DATA MULTIPLE NONSHARED" >> $output_objdir/$libname.def~ $ECHO EXPORTS >> $output_objdir/$libname.def~ emxexp $libobjs | $SED /"_DLL_InitTerm"/d >> $output_objdir/$libname.def~ $CC -Zdll -Zcrtdll -o $output_objdir/$soname $libobjs $deplibs $compiler_flags $output_objdir/$libname.def~ emximp -o $lib $output_objdir/$libname.def' archive_expsym_cmds='$ECHO "LIBRARY ${soname%$shared_ext} INITINSTANCE TERMINSTANCE" > $output_objdir/$libname.def~ $ECHO "DESCRIPTION \"$libname\"" >> $output_objdir/$libname.def~ $ECHO "DATA MULTIPLE NONSHARED" >> $output_objdir/$libname.def~ $ECHO EXPORTS >> $output_objdir/$libname.def~ prefix_cmds="$SED"~ if test EXPORTS = "`$SED 1q $export_symbols`"; then prefix_cmds="$prefix_cmds -e 1d"; fi~ prefix_cmds="$prefix_cmds -e \"s/^\(.*\)$/_\1/g\""~ cat $export_symbols | $prefix_cmds >> $output_objdir/$libname.def~ $CC -Zdll -Zcrtdll -o $output_objdir/$soname $libobjs $deplibs $compiler_flags $output_objdir/$libname.def~ emximp -o $lib $output_objdir/$libname.def' old_archive_From_new_cmds='emximp -o $output_objdir/${libname}_dll.a $output_objdir/$libname.def' enable_shared_with_static_runtimes=yes ;; interix[3-9]*) hardcode_direct=no hardcode_shlibpath_var=no hardcode_libdir_flag_spec='$wl-rpath,$libdir' export_dynamic_flag_spec='$wl-E' # Hack: On Interix 3.x, we cannot compile PIC because of a broken gcc. # Instead, shared libraries are loaded at an image base (0x10000000 by # default) and relocated if they conflict, which is a slow very memory # consuming and fragmenting process. To avoid this, we pick a random, # 256 KiB-aligned image base between 0x50000000 and 0x6FFC0000 at link # time. Moving up from 0x10000000 also allows more sbrk(2) space. archive_cmds='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-h,$soname $wl--image-base,`expr ${RANDOM-$$} % 4096 / 2 \* 262144 + 1342177280` -o $lib' archive_expsym_cmds='sed "s|^|_|" $export_symbols >$output_objdir/$soname.expsym~$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-h,$soname $wl--retain-symbols-file,$output_objdir/$soname.expsym $wl--image-base,`expr ${RANDOM-$$} % 4096 / 2 \* 262144 + 1342177280` -o $lib' ;; gnu* | linux* | tpf* | k*bsd*-gnu | kopensolaris*-gnu) tmp_diet=no if test linux-dietlibc = "$host_os"; then case $cc_basename in diet\ *) tmp_diet=yes;; # linux-dietlibc with static linking (!diet-dyn) esac fi if $LD --help 2>&1 | $EGREP ': supported targets:.* elf' > /dev/null \ && test no = "$tmp_diet" then tmp_addflag=' $pic_flag' tmp_sharedflag='-shared' case $cc_basename,$host_cpu in pgcc*) # Portland Group C compiler whole_archive_flag_spec='$wl--whole-archive`for conv in $convenience\"\"; do test -n \"$conv\" && new_convenience=\"$new_convenience,$conv\"; done; func_echo_all \"$new_convenience\"` $wl--no-whole-archive' tmp_addflag=' $pic_flag' ;; pgf77* | pgf90* | pgf95* | pgfortran*) # Portland Group f77 and f90 compilers whole_archive_flag_spec='$wl--whole-archive`for conv in $convenience\"\"; do test -n \"$conv\" && new_convenience=\"$new_convenience,$conv\"; done; func_echo_all \"$new_convenience\"` $wl--no-whole-archive' tmp_addflag=' $pic_flag -Mnomain' ;; ecc*,ia64* | icc*,ia64*) # Intel C compiler on ia64 tmp_addflag=' -i_dynamic' ;; efc*,ia64* | ifort*,ia64*) # Intel Fortran compiler on ia64 tmp_addflag=' -i_dynamic -nofor_main' ;; ifc* | ifort*) # Intel Fortran compiler tmp_addflag=' -nofor_main' ;; lf95*) # Lahey Fortran 8.1 whole_archive_flag_spec= tmp_sharedflag='--shared' ;; nagfor*) # NAGFOR 5.3 tmp_sharedflag='-Wl,-shared' ;; xl[cC]* | bgxl[cC]* | mpixl[cC]*) # IBM XL C 8.0 on PPC (deal with xlf below) tmp_sharedflag='-qmkshrobj' tmp_addflag= ;; nvcc*) # Cuda Compiler Driver 2.2 whole_archive_flag_spec='$wl--whole-archive`for conv in $convenience\"\"; do test -n \"$conv\" && new_convenience=\"$new_convenience,$conv\"; done; func_echo_all \"$new_convenience\"` $wl--no-whole-archive' compiler_needs_object=yes ;; esac case `$CC -V 2>&1 | sed 5q` in *Sun\ C*) # Sun C 5.9 whole_archive_flag_spec='$wl--whole-archive`new_convenience=; for conv in $convenience\"\"; do test -z \"$conv\" || new_convenience=\"$new_convenience,$conv\"; done; func_echo_all \"$new_convenience\"` $wl--no-whole-archive' compiler_needs_object=yes tmp_sharedflag='-G' ;; *Sun\ F*) # Sun Fortran 8.3 tmp_sharedflag='-G' ;; esac archive_cmds='$CC '"$tmp_sharedflag""$tmp_addflag"' $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' if test yes = "$supports_anon_versioning"; then archive_expsym_cmds='echo "{ global:" > $output_objdir/$libname.ver~ cat $export_symbols | sed -e "s/\(.*\)/\1;/" >> $output_objdir/$libname.ver~ echo "local: *; };" >> $output_objdir/$libname.ver~ $CC '"$tmp_sharedflag""$tmp_addflag"' $libobjs $deplibs $compiler_flags $wl-soname $wl$soname $wl-version-script $wl$output_objdir/$libname.ver -o $lib' fi case $cc_basename in tcc*) export_dynamic_flag_spec='-rdynamic' ;; xlf* | bgf* | bgxlf* | mpixlf*) # IBM XL Fortran 10.1 on PPC cannot create shared libs itself whole_archive_flag_spec='--whole-archive$convenience --no-whole-archive' hardcode_libdir_flag_spec='$wl-rpath $wl$libdir' archive_cmds='$LD -shared $libobjs $deplibs $linker_flags -soname $soname -o $lib' if test yes = "$supports_anon_versioning"; then archive_expsym_cmds='echo "{ global:" > $output_objdir/$libname.ver~ cat $export_symbols | sed -e "s/\(.*\)/\1;/" >> $output_objdir/$libname.ver~ echo "local: *; };" >> $output_objdir/$libname.ver~ $LD -shared $libobjs $deplibs $linker_flags -soname $soname -version-script $output_objdir/$libname.ver -o $lib' fi ;; esac else ld_shlibs=no fi ;; netbsd*) if echo __ELF__ | $CC -E - | $GREP __ELF__ >/dev/null; then archive_cmds='$LD -Bshareable $libobjs $deplibs $linker_flags -o $lib' wlarc= else archive_cmds='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' archive_expsym_cmds='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname $wl-retain-symbols-file $wl$export_symbols -o $lib' fi ;; solaris*) if $LD -v 2>&1 | $GREP 'BFD 2\.8' > /dev/null; then ld_shlibs=no cat <<_LT_EOF 1>&2 *** Warning: The releases 2.8.* of the GNU linker cannot reliably *** create shared libraries on Solaris systems. Therefore, libtool *** is disabling shared libraries support. We urge you to upgrade GNU *** binutils to release 2.9.1 or newer. Another option is to modify *** your PATH or compiler configuration so that the native linker is *** used, and then restart. _LT_EOF elif $LD --help 2>&1 | $GREP ': supported targets:.* elf' > /dev/null; then archive_cmds='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' archive_expsym_cmds='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname $wl-retain-symbols-file $wl$export_symbols -o $lib' else ld_shlibs=no fi ;; sysv5* | sco3.2v5* | sco5v6* | unixware* | OpenUNIX*) case `$LD -v 2>&1` in *\ [01].* | *\ 2.[0-9].* | *\ 2.1[0-5].*) ld_shlibs=no cat <<_LT_EOF 1>&2 *** Warning: Releases of the GNU linker prior to 2.16.91.0.3 cannot *** reliably create shared libraries on SCO systems. Therefore, libtool *** is disabling shared libraries support. We urge you to upgrade GNU *** binutils to release 2.16.91.0.3 or newer. Another option is to modify *** your PATH or compiler configuration so that the native linker is *** used, and then restart. _LT_EOF ;; *) # For security reasons, it is highly recommended that you always # use absolute paths for naming shared libraries, and exclude the # DT_RUNPATH tag from executables and libraries. But doing so # requires that you compile everything twice, which is a pain. if $LD --help 2>&1 | $GREP ': supported targets:.* elf' > /dev/null; then hardcode_libdir_flag_spec='$wl-rpath $wl$libdir' archive_cmds='$CC -shared $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' archive_expsym_cmds='$CC -shared $libobjs $deplibs $compiler_flags $wl-soname $wl$soname $wl-retain-symbols-file $wl$export_symbols -o $lib' else ld_shlibs=no fi ;; esac ;; sunos4*) archive_cmds='$LD -assert pure-text -Bshareable -o $lib $libobjs $deplibs $linker_flags' wlarc= hardcode_direct=yes hardcode_shlibpath_var=no ;; *) if $LD --help 2>&1 | $GREP ': supported targets:.* elf' > /dev/null; then archive_cmds='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' archive_expsym_cmds='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname $wl-retain-symbols-file $wl$export_symbols -o $lib' else ld_shlibs=no fi ;; esac if test no = "$ld_shlibs"; then runpath_var= hardcode_libdir_flag_spec= export_dynamic_flag_spec= whole_archive_flag_spec= fi else # PORTME fill in a description of your system's linker (not GNU ld) case $host_os in aix3*) allow_undefined_flag=unsupported always_export_symbols=yes archive_expsym_cmds='$LD -o $output_objdir/$soname $libobjs $deplibs $linker_flags -bE:$export_symbols -T512 -H512 -bM:SRE~$AR $AR_FLAGS $lib $output_objdir/$soname' # Note: this linker hardcodes the directories in LIBPATH if there # are no directories specified by -L. hardcode_minus_L=yes if test yes = "$GCC" && test -z "$lt_prog_compiler_static"; then # Neither direct hardcoding nor static linking is supported with a # broken collect2. hardcode_direct=unsupported fi ;; aix[4-9]*) if test ia64 = "$host_cpu"; then # On IA64, the linker does run time linking by default, so we don't # have to do anything special. aix_use_runtimelinking=no exp_sym_flag='-Bexport' no_entry_flag= else # If we're using GNU nm, then we don't want the "-C" option. # -C means demangle to GNU nm, but means don't demangle to AIX nm. # Without the "-l" option, or with the "-B" option, AIX nm treats # weak defined symbols like other global defined symbols, whereas # GNU nm marks them as "W". # While the 'weak' keyword is ignored in the Export File, we need # it in the Import File for the 'aix-soname' feature, so we have # to replace the "-B" option with "-P" for AIX nm. if $NM -V 2>&1 | $GREP 'GNU' > /dev/null; then export_symbols_cmds='$NM -Bpg $libobjs $convenience | awk '\''{ if (((\$ 2 == "T") || (\$ 2 == "D") || (\$ 2 == "B") || (\$ 2 == "W")) && (substr(\$ 3,1,1) != ".")) { if (\$ 2 == "W") { print \$ 3 " weak" } else { print \$ 3 } } }'\'' | sort -u > $export_symbols' else export_symbols_cmds='`func_echo_all $NM | $SED -e '\''s/B\([^B]*\)$/P\1/'\''` -PCpgl $libobjs $convenience | awk '\''{ if (((\$ 2 == "T") || (\$ 2 == "D") || (\$ 2 == "B") || (\$ 2 == "W") || (\$ 2 == "V") || (\$ 2 == "Z")) && (substr(\$ 1,1,1) != ".")) { if ((\$ 2 == "W") || (\$ 2 == "V") || (\$ 2 == "Z")) { print \$ 1 " weak" } else { print \$ 1 } } }'\'' | sort -u > $export_symbols' fi aix_use_runtimelinking=no # Test if we are trying to use run time linking or normal # AIX style linking. If -brtl is somewhere in LDFLAGS, we # have runtime linking enabled, and use it for executables. # For shared libraries, we enable/disable runtime linking # depending on the kind of the shared library created - # when "with_aix_soname,aix_use_runtimelinking" is: # "aix,no" lib.a(lib.so.V) shared, rtl:no, for executables # "aix,yes" lib.so shared, rtl:yes, for executables # lib.a static archive # "both,no" lib.so.V(shr.o) shared, rtl:yes # lib.a(lib.so.V) shared, rtl:no, for executables # "both,yes" lib.so.V(shr.o) shared, rtl:yes, for executables # lib.a(lib.so.V) shared, rtl:no # "svr4,*" lib.so.V(shr.o) shared, rtl:yes, for executables # lib.a static archive case $host_os in aix4.[23]|aix4.[23].*|aix[5-9]*) for ld_flag in $LDFLAGS; do if (test x-brtl = "x$ld_flag" || test x-Wl,-brtl = "x$ld_flag"); then aix_use_runtimelinking=yes break fi done if test svr4,no = "$with_aix_soname,$aix_use_runtimelinking"; then # With aix-soname=svr4, we create the lib.so.V shared archives only, # so we don't have lib.a shared libs to link our executables. # We have to force runtime linking in this case. aix_use_runtimelinking=yes LDFLAGS="$LDFLAGS -Wl,-brtl" fi ;; esac exp_sym_flag='-bexport' no_entry_flag='-bnoentry' fi # When large executables or shared objects are built, AIX ld can # have problems creating the table of contents. If linking a library # or program results in "error TOC overflow" add -mminimal-toc to # CXXFLAGS/CFLAGS for g++/gcc. In the cases where that is not # enough to fix the problem, add -Wl,-bbigtoc to LDFLAGS. archive_cmds='' hardcode_direct=yes hardcode_direct_absolute=yes hardcode_libdir_separator=':' link_all_deplibs=yes file_list_spec='$wl-f,' case $with_aix_soname,$aix_use_runtimelinking in aix,*) ;; # traditional, no import file svr4,* | *,yes) # use import file # The Import File defines what to hardcode. hardcode_direct=no hardcode_direct_absolute=no ;; esac if test yes = "$GCC"; then case $host_os in aix4.[012]|aix4.[012].*) # We only want to do this on AIX 4.2 and lower, the check # below for broken collect2 doesn't work under 4.3+ collect2name=`$CC -print-prog-name=collect2` if test -f "$collect2name" && strings "$collect2name" | $GREP resolve_lib_name >/dev/null then # We have reworked collect2 : else # We have old collect2 hardcode_direct=unsupported # It fails to find uninstalled libraries when the uninstalled # path is not listed in the libpath. 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then : lt_aix_libpath_sed=' /Import File Strings/,/^$/ { /^0/ { s/^0 *\([^ ]*\) *$/\1/ p } }' lt_cv_aix_libpath_=`dump -H conftest$ac_exeext 2>/dev/null | $SED -n -e "$lt_aix_libpath_sed"` # Check for a 64-bit object if we didn't find anything. if test -z "$lt_cv_aix_libpath_"; then lt_cv_aix_libpath_=`dump -HX64 conftest$ac_exeext 2>/dev/null | $SED -n -e "$lt_aix_libpath_sed"` fi fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext if test -z "$lt_cv_aix_libpath_"; then lt_cv_aix_libpath_=/usr/lib:/lib fi fi aix_libpath=$lt_cv_aix_libpath_ fi hardcode_libdir_flag_spec='$wl-blibpath:$libdir:'"$aix_libpath" archive_expsym_cmds='$CC -o $output_objdir/$soname $libobjs $deplibs $wl'$no_entry_flag' $compiler_flags `if test -n "$allow_undefined_flag"; then func_echo_all "$wl$allow_undefined_flag"; else :; fi` $wl'$exp_sym_flag:\$export_symbols' '$shared_flag else if test ia64 = "$host_cpu"; then hardcode_libdir_flag_spec='$wl-R $libdir:/usr/lib:/lib' allow_undefined_flag="-z nodefs" archive_expsym_cmds="\$CC $shared_flag"' -o $output_objdir/$soname $libobjs $deplibs '"\$wl$no_entry_flag"' $compiler_flags $wl$allow_undefined_flag '"\$wl$exp_sym_flag:\$export_symbols" else # Determine the default libpath from the value encoded in an # empty executable. if test set = "${lt_cv_aix_libpath+set}"; then aix_libpath=$lt_cv_aix_libpath else if ${lt_cv_aix_libpath_+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ int main () { ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : lt_aix_libpath_sed=' /Import File Strings/,/^$/ { /^0/ { s/^0 *\([^ ]*\) *$/\1/ p } }' lt_cv_aix_libpath_=`dump -H conftest$ac_exeext 2>/dev/null | $SED -n -e "$lt_aix_libpath_sed"` # Check for a 64-bit object if we didn't find anything. if test -z "$lt_cv_aix_libpath_"; then lt_cv_aix_libpath_=`dump -HX64 conftest$ac_exeext 2>/dev/null | $SED -n -e "$lt_aix_libpath_sed"` fi fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext if test -z "$lt_cv_aix_libpath_"; then lt_cv_aix_libpath_=/usr/lib:/lib fi fi aix_libpath=$lt_cv_aix_libpath_ fi hardcode_libdir_flag_spec='$wl-blibpath:$libdir:'"$aix_libpath" # Warning - without using the other run time loading flags, # -berok will link without error, but may produce a broken library. no_undefined_flag=' $wl-bernotok' allow_undefined_flag=' $wl-berok' if test yes = "$with_gnu_ld"; then # We only use this code for GNU lds that support --whole-archive. whole_archive_flag_spec='$wl--whole-archive$convenience $wl--no-whole-archive' else # Exported symbols can be pulled into shared objects from archives whole_archive_flag_spec='$convenience' fi archive_cmds_need_lc=yes archive_expsym_cmds='$RM -r $output_objdir/$realname.d~$MKDIR $output_objdir/$realname.d' # -brtl affects multiple linker settings, -berok does not and is overridden later compiler_flags_filtered='`func_echo_all "$compiler_flags " | $SED -e "s%-brtl\\([, ]\\)%-berok\\1%g"`' if test svr4 != "$with_aix_soname"; then # This is similar to how AIX traditionally builds its shared libraries. archive_expsym_cmds="$archive_expsym_cmds"'~$CC '$shared_flag_aix' -o $output_objdir/$realname.d/$soname $libobjs $deplibs $wl-bnoentry '$compiler_flags_filtered'$wl-bE:$export_symbols$allow_undefined_flag~$AR $AR_FLAGS $output_objdir/$libname$release.a $output_objdir/$realname.d/$soname' fi if test aix != "$with_aix_soname"; then archive_expsym_cmds="$archive_expsym_cmds"'~$CC '$shared_flag_svr4' -o $output_objdir/$realname.d/$shared_archive_member_spec.o $libobjs $deplibs $wl-bnoentry '$compiler_flags_filtered'$wl-bE:$export_symbols$allow_undefined_flag~$STRIP -e $output_objdir/$realname.d/$shared_archive_member_spec.o~( func_echo_all "#! $soname($shared_archive_member_spec.o)"; if test shr_64 = "$shared_archive_member_spec"; then func_echo_all "# 64"; else func_echo_all "# 32"; fi; cat $export_symbols ) > $output_objdir/$realname.d/$shared_archive_member_spec.imp~$AR $AR_FLAGS $output_objdir/$soname $output_objdir/$realname.d/$shared_archive_member_spec.o $output_objdir/$realname.d/$shared_archive_member_spec.imp' else # used by -dlpreopen to get the symbols archive_expsym_cmds="$archive_expsym_cmds"'~$MV $output_objdir/$realname.d/$soname $output_objdir' fi archive_expsym_cmds="$archive_expsym_cmds"'~$RM -r $output_objdir/$realname.d' fi fi ;; amigaos*) case $host_cpu in powerpc) # see comment about AmigaOS4 .so support archive_cmds='$CC -shared $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' archive_expsym_cmds='' ;; m68k) archive_cmds='$RM $output_objdir/a2ixlibrary.data~$ECHO "#define NAME $libname" > $output_objdir/a2ixlibrary.data~$ECHO "#define LIBRARY_ID 1" >> $output_objdir/a2ixlibrary.data~$ECHO "#define VERSION $major" >> $output_objdir/a2ixlibrary.data~$ECHO "#define REVISION $revision" >> $output_objdir/a2ixlibrary.data~$AR $AR_FLAGS $lib $libobjs~$RANLIB $lib~(cd $output_objdir && a2ixlibrary -32)' hardcode_libdir_flag_spec='-L$libdir' hardcode_minus_L=yes ;; esac ;; bsdi[45]*) export_dynamic_flag_spec=-rdynamic ;; cygwin* | mingw* | pw32* | cegcc*) # When not using gcc, we currently assume that we are using # Microsoft Visual C++. # hardcode_libdir_flag_spec is actually meaningless, as there is # no search path for DLLs. case $cc_basename in cl*) # Native MSVC hardcode_libdir_flag_spec=' ' allow_undefined_flag=unsupported always_export_symbols=yes file_list_spec='@' # Tell ltmain to make .lib files, not .a files. libext=lib # Tell ltmain to make .dll files, not .so files. shrext_cmds=.dll # FIXME: Setting linknames here is a bad hack. archive_cmds='$CC -o $output_objdir/$soname $libobjs $compiler_flags $deplibs -Wl,-DLL,-IMPLIB:"$tool_output_objdir$libname.dll.lib"~linknames=' archive_expsym_cmds='if test DEF = "`$SED -n -e '\''s/^[ ]*//'\'' -e '\''/^\(;.*\)*$/d'\'' -e '\''s/^\(EXPORTS\|LIBRARY\)\([ ].*\)*$/DEF/p'\'' -e q $export_symbols`" ; then cp "$export_symbols" "$output_objdir/$soname.def"; echo "$tool_output_objdir$soname.def" > "$output_objdir/$soname.exp"; else $SED -e '\''s/^/-link -EXPORT:/'\'' < $export_symbols > $output_objdir/$soname.exp; fi~ $CC -o $tool_output_objdir$soname $libobjs $compiler_flags $deplibs "@$tool_output_objdir$soname.exp" -Wl,-DLL,-IMPLIB:"$tool_output_objdir$libname.dll.lib"~ linknames=' # The linker will not automatically build a static lib if we build a DLL. # _LT_TAGVAR(old_archive_from_new_cmds, )='true' enable_shared_with_static_runtimes=yes exclude_expsyms='_NULL_IMPORT_DESCRIPTOR|_IMPORT_DESCRIPTOR_.*' export_symbols_cmds='$NM $libobjs $convenience | $global_symbol_pipe | $SED -e '\''/^[BCDGRS][ ]/s/.*[ ]\([^ ]*\)/\1,DATA/'\'' | $SED -e '\''/^[AITW][ ]/s/.*[ ]//'\'' | sort | uniq > $export_symbols' # Don't use ranlib old_postinstall_cmds='chmod 644 $oldlib' postlink_cmds='lt_outputfile="@OUTPUT@"~ lt_tool_outputfile="@TOOL_OUTPUT@"~ case $lt_outputfile in *.exe|*.EXE) ;; *) lt_outputfile=$lt_outputfile.exe lt_tool_outputfile=$lt_tool_outputfile.exe ;; esac~ if test : != "$MANIFEST_TOOL" && test -f "$lt_outputfile.manifest"; then $MANIFEST_TOOL -manifest "$lt_tool_outputfile.manifest" -outputresource:"$lt_tool_outputfile" || exit 1; $RM "$lt_outputfile.manifest"; fi' ;; *) # Assume MSVC wrapper hardcode_libdir_flag_spec=' ' allow_undefined_flag=unsupported # Tell ltmain to make .lib files, not .a files. libext=lib # Tell ltmain to make .dll files, not .so files. shrext_cmds=.dll # FIXME: Setting linknames here is a bad hack. archive_cmds='$CC -o $lib $libobjs $compiler_flags `func_echo_all "$deplibs" | $SED '\''s/ -lc$//'\''` -link -dll~linknames=' # The linker will automatically build a .lib file if we build a DLL. old_archive_from_new_cmds='true' # FIXME: Should let the user specify the lib program. old_archive_cmds='lib -OUT:$oldlib$oldobjs$old_deplibs' enable_shared_with_static_runtimes=yes ;; esac ;; darwin* | rhapsody*) archive_cmds_need_lc=no hardcode_direct=no hardcode_automatic=yes hardcode_shlibpath_var=unsupported if test yes = "$lt_cv_ld_force_load"; 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dgux*) archive_cmds='$LD -G -h $soname -o $lib $libobjs $deplibs $linker_flags' hardcode_libdir_flag_spec='-L$libdir' hardcode_shlibpath_var=no ;; # FreeBSD 2.2.[012] allows us to include c++rt0.o to get C++ constructor # support. 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linux*) case $cc_basename in tcc*) # Fabrice Bellard et al's Tiny C Compiler ld_shlibs=yes archive_cmds='$CC -shared $pic_flag -o $lib $libobjs $deplibs $compiler_flags' ;; esac ;; netbsd*) if echo __ELF__ | $CC -E - | $GREP __ELF__ >/dev/null; then archive_cmds='$LD -Bshareable -o $lib $libobjs $deplibs $linker_flags' # a.out else archive_cmds='$LD -shared -o $lib $libobjs $deplibs $linker_flags' # ELF fi hardcode_libdir_flag_spec='-R$libdir' hardcode_direct=yes hardcode_shlibpath_var=no ;; newsos6) archive_cmds='$LD -G -h $soname -o $lib $libobjs $deplibs $linker_flags' hardcode_direct=yes hardcode_libdir_flag_spec='$wl-rpath $wl$libdir' hardcode_libdir_separator=: hardcode_shlibpath_var=no ;; *nto* | *qnx*) ;; openbsd* | bitrig*) if test -f /usr/libexec/ld.so; then hardcode_direct=yes hardcode_shlibpath_var=no hardcode_direct_absolute=yes if test -z "`echo __ELF__ | $CC -E - | $GREP __ELF__`"; then archive_cmds='$CC -shared $pic_flag -o $lib $libobjs $deplibs $compiler_flags' archive_expsym_cmds='$CC -shared $pic_flag -o $lib $libobjs $deplibs $compiler_flags $wl-retain-symbols-file,$export_symbols' hardcode_libdir_flag_spec='$wl-rpath,$libdir' export_dynamic_flag_spec='$wl-E' else archive_cmds='$CC -shared $pic_flag -o $lib $libobjs $deplibs $compiler_flags' hardcode_libdir_flag_spec='$wl-rpath,$libdir' fi else ld_shlibs=no fi ;; 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When/if they implement a new # versioning mechanism, adjust this. if test -x /usr/bin/objformat; then objformat=`/usr/bin/objformat` else case $host_os in freebsd[23].*) objformat=aout ;; *) objformat=elf ;; esac fi version_type=freebsd-$objformat case $version_type in freebsd-elf*) library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' need_version=no need_lib_prefix=no ;; freebsd-*) library_names_spec='$libname$release$shared_ext$versuffix $libname$shared_ext$versuffix' need_version=yes ;; esac shlibpath_var=LD_LIBRARY_PATH case $host_os in freebsd2.*) shlibpath_overrides_runpath=yes ;; freebsd3.[01]* | freebsdelf3.[01]*) shlibpath_overrides_runpath=yes hardcode_into_libs=yes ;; freebsd3.[2-9]* | freebsdelf3.[2-9]* | \ freebsd4.[0-5] | freebsdelf4.[0-5] | freebsd4.1.1 | freebsdelf4.1.1) shlibpath_overrides_runpath=no hardcode_into_libs=yes ;; *) # from 4.6 on, and DragonFly shlibpath_overrides_runpath=yes hardcode_into_libs=yes ;; esac ;; haiku*) version_type=linux # correct to gnu/linux during the next big refactor need_lib_prefix=no need_version=no dynamic_linker="$host_os runtime_loader" library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' shlibpath_var=LIBRARY_PATH shlibpath_overrides_runpath=no sys_lib_dlsearch_path_spec='/boot/home/config/lib /boot/common/lib /boot/system/lib' hardcode_into_libs=yes ;; hpux9* | hpux10* | hpux11*) # Give a soname corresponding to the major version so that dld.sl refuses to # link against other versions. version_type=sunos need_lib_prefix=no need_version=no case $host_cpu in ia64*) shrext_cmds='.so' hardcode_into_libs=yes dynamic_linker="$host_os dld.so" shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes # Unless +noenvvar is specified. library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' if test 32 = "$HPUX_IA64_MODE"; then sys_lib_search_path_spec="/usr/lib/hpux32 /usr/local/lib/hpux32 /usr/local/lib" sys_lib_dlsearch_path_spec=/usr/lib/hpux32 else sys_lib_search_path_spec="/usr/lib/hpux64 /usr/local/lib/hpux64" sys_lib_dlsearch_path_spec=/usr/lib/hpux64 fi ;; hppa*64*) shrext_cmds='.sl' hardcode_into_libs=yes dynamic_linker="$host_os dld.sl" shlibpath_var=LD_LIBRARY_PATH # How should we handle SHLIB_PATH shlibpath_overrides_runpath=yes # Unless +noenvvar is specified. library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' sys_lib_search_path_spec="/usr/lib/pa20_64 /usr/ccs/lib/pa20_64" sys_lib_dlsearch_path_spec=$sys_lib_search_path_spec ;; *) shrext_cmds='.sl' dynamic_linker="$host_os dld.sl" shlibpath_var=SHLIB_PATH shlibpath_overrides_runpath=no # +s is required to enable SHLIB_PATH library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' ;; esac # HP-UX runs *really* slowly unless shared libraries are mode 555, ... postinstall_cmds='chmod 555 $lib' # or fails outright, so override atomically: install_override_mode=555 ;; interix[3-9]*) version_type=linux # correct to gnu/linux during the next big refactor need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' dynamic_linker='Interix 3.x ld.so.1 (PE, like ELF)' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=no hardcode_into_libs=yes ;; irix5* | irix6* | nonstopux*) case $host_os in nonstopux*) version_type=nonstopux ;; *) if test yes = "$lt_cv_prog_gnu_ld"; then version_type=linux # correct to gnu/linux during the next big refactor else version_type=irix fi ;; esac need_lib_prefix=no need_version=no soname_spec='$libname$release$shared_ext$major' library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$release$shared_ext $libname$shared_ext' case $host_os in irix5* | nonstopux*) libsuff= shlibsuff= ;; *) case $LD in # libtool.m4 will add one of these switches to LD *-32|*"-32 "|*-melf32bsmip|*"-melf32bsmip ") libsuff= shlibsuff= libmagic=32-bit;; *-n32|*"-n32 "|*-melf32bmipn32|*"-melf32bmipn32 ") libsuff=32 shlibsuff=N32 libmagic=N32;; *-64|*"-64 "|*-melf64bmip|*"-melf64bmip ") libsuff=64 shlibsuff=64 libmagic=64-bit;; *) libsuff= shlibsuff= libmagic=never-match;; esac ;; esac shlibpath_var=LD_LIBRARY${shlibsuff}_PATH shlibpath_overrides_runpath=no sys_lib_search_path_spec="/usr/lib$libsuff /lib$libsuff /usr/local/lib$libsuff" sys_lib_dlsearch_path_spec="/usr/lib$libsuff /lib$libsuff" hardcode_into_libs=yes ;; # No shared lib support for Linux oldld, aout, or coff. linux*oldld* | linux*aout* | linux*coff*) dynamic_linker=no ;; linux*android*) version_type=none # Android doesn't support versioned libraries. need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext' soname_spec='$libname$release$shared_ext' finish_cmds= shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes # This implies no fast_install, which is unacceptable. # Some rework will be needed to allow for fast_install # before this can be enabled. hardcode_into_libs=yes dynamic_linker='Android linker' # Don't embed -rpath directories since the linker doesn't support them. hardcode_libdir_flag_spec='-L$libdir' ;; # This must be glibc/ELF. linux* | k*bsd*-gnu | kopensolaris*-gnu | gnu*) version_type=linux # correct to gnu/linux during the next big refactor need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' finish_cmds='PATH="\$PATH:/sbin" ldconfig -n $libdir' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=no # Some binutils ld are patched to set DT_RUNPATH if ${lt_cv_shlibpath_overrides_runpath+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_shlibpath_overrides_runpath=no save_LDFLAGS=$LDFLAGS save_libdir=$libdir eval "libdir=/foo; wl=\"$lt_prog_compiler_wl\"; \ LDFLAGS=\"\$LDFLAGS $hardcode_libdir_flag_spec\"" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ int main () { ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : if ($OBJDUMP -p conftest$ac_exeext) 2>/dev/null | grep "RUNPATH.*$libdir" >/dev/null; then : lt_cv_shlibpath_overrides_runpath=yes fi fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LDFLAGS=$save_LDFLAGS libdir=$save_libdir fi shlibpath_overrides_runpath=$lt_cv_shlibpath_overrides_runpath # This implies no fast_install, which is unacceptable. # Some rework will be needed to allow for fast_install # before this can be enabled. hardcode_into_libs=yes # Ideally, we could use ldconfig to report *all* directores which are # searched for libraries, however this is still not possible. Aside from not # being certain /sbin/ldconfig is available, command # 'ldconfig -N -X -v | grep ^/' on 64bit Fedora does not report /usr/lib64, # even though it is searched at run-time. Try to do the best guess by # appending ld.so.conf contents (and includes) to the search path. if test -f /etc/ld.so.conf; then lt_ld_extra=`awk '/^include / { system(sprintf("cd /etc; cat %s 2>/dev/null", \$2)); skip = 1; } { if (!skip) print \$0; skip = 0; }' < /etc/ld.so.conf | $SED -e 's/#.*//;/^[ ]*hwcap[ ]/d;s/[:, ]/ /g;s/=[^=]*$//;s/=[^= ]* / /g;s/"//g;/^$/d' | tr '\n' ' '` sys_lib_dlsearch_path_spec="/lib /usr/lib $lt_ld_extra" fi # We used to test for /lib/ld.so.1 and disable shared libraries on # powerpc, because MkLinux only supported shared libraries with the # GNU dynamic linker. Since this was broken with cross compilers, # most powerpc-linux boxes support dynamic linking these days and # people can always --disable-shared, the test was removed, and we # assume the GNU/Linux dynamic linker is in use. dynamic_linker='GNU/Linux ld.so' ;; netbsd*) version_type=sunos need_lib_prefix=no need_version=no if echo __ELF__ | $CC -E - | $GREP __ELF__ >/dev/null; then library_names_spec='$libname$release$shared_ext$versuffix $libname$shared_ext$versuffix' finish_cmds='PATH="\$PATH:/sbin" ldconfig -m $libdir' dynamic_linker='NetBSD (a.out) ld.so' else library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' dynamic_linker='NetBSD ld.elf_so' fi shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes hardcode_into_libs=yes ;; newsos6) version_type=linux # correct to gnu/linux during the next big refactor library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes ;; *nto* | *qnx*) version_type=qnx need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=no hardcode_into_libs=yes dynamic_linker='ldqnx.so' ;; openbsd* | bitrig*) version_type=sunos sys_lib_dlsearch_path_spec=/usr/lib need_lib_prefix=no if test -z "`echo __ELF__ | $CC -E - | $GREP __ELF__`"; then need_version=no else need_version=yes fi library_names_spec='$libname$release$shared_ext$versuffix $libname$shared_ext$versuffix' finish_cmds='PATH="\$PATH:/sbin" ldconfig -m $libdir' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes ;; os2*) libname_spec='$name' version_type=windows shrext_cmds=.dll need_version=no need_lib_prefix=no # OS/2 can only load a DLL with a base name of 8 characters or less. soname_spec='`test -n "$os2dllname" && libname="$os2dllname"; v=$($ECHO $release$versuffix | tr -d .-); n=$($ECHO $libname | cut -b -$((8 - ${#v})) | tr . _); $ECHO $n$v`$shared_ext' library_names_spec='${libname}_dll.$libext' dynamic_linker='OS/2 ld.exe' shlibpath_var=BEGINLIBPATH sys_lib_search_path_spec="/lib /usr/lib /usr/local/lib" sys_lib_dlsearch_path_spec=$sys_lib_search_path_spec postinstall_cmds='base_file=`basename \$file`~ dlpath=`$SHELL 2>&1 -c '\''. $dir/'\''\$base_file'\''i; $ECHO \$dlname'\''`~ dldir=$destdir/`dirname \$dlpath`~ test -d \$dldir || mkdir -p \$dldir~ $install_prog $dir/$dlname \$dldir/$dlname~ chmod a+x \$dldir/$dlname~ if test -n '\''$stripme'\'' && test -n '\''$striplib'\''; then eval '\''$striplib \$dldir/$dlname'\'' || exit \$?; fi' postuninstall_cmds='dldll=`$SHELL 2>&1 -c '\''. $file; $ECHO \$dlname'\''`~ dlpath=$dir/\$dldll~ $RM \$dlpath' ;; osf3* | osf4* | osf5*) version_type=osf need_lib_prefix=no need_version=no soname_spec='$libname$release$shared_ext$major' library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' shlibpath_var=LD_LIBRARY_PATH sys_lib_search_path_spec="/usr/shlib /usr/ccs/lib /usr/lib/cmplrs/cc /usr/lib /usr/local/lib /var/shlib" sys_lib_dlsearch_path_spec=$sys_lib_search_path_spec ;; rdos*) dynamic_linker=no ;; solaris*) version_type=linux # correct to gnu/linux during the next big refactor need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes hardcode_into_libs=yes # ldd complains unless libraries are executable postinstall_cmds='chmod +x $lib' ;; sunos4*) version_type=sunos library_names_spec='$libname$release$shared_ext$versuffix $libname$shared_ext$versuffix' finish_cmds='PATH="\$PATH:/usr/etc" ldconfig $libdir' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes if test yes = "$with_gnu_ld"; then need_lib_prefix=no fi need_version=yes ;; sysv4 | sysv4.3*) version_type=linux # correct to gnu/linux during the next big refactor library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' shlibpath_var=LD_LIBRARY_PATH case $host_vendor in sni) shlibpath_overrides_runpath=no need_lib_prefix=no runpath_var=LD_RUN_PATH ;; siemens) need_lib_prefix=no ;; motorola) need_lib_prefix=no need_version=no shlibpath_overrides_runpath=no sys_lib_search_path_spec='/lib /usr/lib /usr/ccs/lib' ;; esac ;; sysv4*MP*) if test -d /usr/nec; then version_type=linux # correct to gnu/linux during the next big refactor library_names_spec='$libname$shared_ext.$versuffix $libname$shared_ext.$major $libname$shared_ext' soname_spec='$libname$shared_ext.$major' shlibpath_var=LD_LIBRARY_PATH fi ;; sysv5* | sco3.2v5* | sco5v6* | unixware* | OpenUNIX* | sysv4*uw2*) version_type=sco need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes hardcode_into_libs=yes if test yes = "$with_gnu_ld"; then sys_lib_search_path_spec='/usr/local/lib /usr/gnu/lib /usr/ccs/lib /usr/lib /lib' else sys_lib_search_path_spec='/usr/ccs/lib /usr/lib' case $host_os in sco3.2v5*) sys_lib_search_path_spec="$sys_lib_search_path_spec /lib" ;; esac fi sys_lib_dlsearch_path_spec='/usr/lib' ;; tpf*) # TPF is a cross-target only. Preferred cross-host = GNU/Linux. version_type=linux # correct to gnu/linux during the next big refactor need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=no hardcode_into_libs=yes ;; uts4*) version_type=linux # correct to gnu/linux during the next big refactor library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' shlibpath_var=LD_LIBRARY_PATH ;; *) dynamic_linker=no ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: result: $dynamic_linker" >&5 $as_echo "$dynamic_linker" >&6; } test no = "$dynamic_linker" && can_build_shared=no variables_saved_for_relink="PATH $shlibpath_var $runpath_var" if test yes = "$GCC"; then variables_saved_for_relink="$variables_saved_for_relink GCC_EXEC_PREFIX COMPILER_PATH LIBRARY_PATH" fi if test set = "${lt_cv_sys_lib_search_path_spec+set}"; then sys_lib_search_path_spec=$lt_cv_sys_lib_search_path_spec fi if test set = "${lt_cv_sys_lib_dlsearch_path_spec+set}"; then sys_lib_dlsearch_path_spec=$lt_cv_sys_lib_dlsearch_path_spec fi # remember unaugmented sys_lib_dlsearch_path content for libtool script decls... configure_time_dlsearch_path=$sys_lib_dlsearch_path_spec # ... but it needs LT_SYS_LIBRARY_PATH munging for other configure-time code func_munge_path_list sys_lib_dlsearch_path_spec "$LT_SYS_LIBRARY_PATH" # to be used as default LT_SYS_LIBRARY_PATH value in generated libtool configure_time_lt_sys_library_path=$LT_SYS_LIBRARY_PATH { $as_echo "$as_me:${as_lineno-$LINENO}: checking how to hardcode library paths into programs" >&5 $as_echo_n "checking how to hardcode library paths into programs... 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esac ac_fn_c_check_decl "$LINENO" "clearerr_unlocked" "ac_cv_have_decl_clearerr_unlocked" "$ac_includes_default" if test "x$ac_cv_have_decl_clearerr_unlocked" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_CLEARERR_UNLOCKED $ac_have_decl _ACEOF ac_fn_c_check_decl "$LINENO" "feof_unlocked" "ac_cv_have_decl_feof_unlocked" "$ac_includes_default" if test "x$ac_cv_have_decl_feof_unlocked" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_FEOF_UNLOCKED $ac_have_decl _ACEOF ac_fn_c_check_decl "$LINENO" "ferror_unlocked" "ac_cv_have_decl_ferror_unlocked" "$ac_includes_default" if test "x$ac_cv_have_decl_ferror_unlocked" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_FERROR_UNLOCKED $ac_have_decl _ACEOF ac_fn_c_check_decl "$LINENO" "fflush_unlocked" "ac_cv_have_decl_fflush_unlocked" "$ac_includes_default" if test "x$ac_cv_have_decl_fflush_unlocked" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_FFLUSH_UNLOCKED $ac_have_decl _ACEOF ac_fn_c_check_decl "$LINENO" "fgets_unlocked" "ac_cv_have_decl_fgets_unlocked" "$ac_includes_default" if test "x$ac_cv_have_decl_fgets_unlocked" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_FGETS_UNLOCKED $ac_have_decl _ACEOF ac_fn_c_check_decl "$LINENO" "fputc_unlocked" "ac_cv_have_decl_fputc_unlocked" "$ac_includes_default" if test "x$ac_cv_have_decl_fputc_unlocked" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_FPUTC_UNLOCKED $ac_have_decl _ACEOF ac_fn_c_check_decl "$LINENO" "fputs_unlocked" "ac_cv_have_decl_fputs_unlocked" "$ac_includes_default" if test "x$ac_cv_have_decl_fputs_unlocked" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_FPUTS_UNLOCKED $ac_have_decl _ACEOF ac_fn_c_check_decl "$LINENO" "fread_unlocked" "ac_cv_have_decl_fread_unlocked" "$ac_includes_default" if test "x$ac_cv_have_decl_fread_unlocked" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_FREAD_UNLOCKED $ac_have_decl _ACEOF ac_fn_c_check_decl "$LINENO" "fwrite_unlocked" "ac_cv_have_decl_fwrite_unlocked" "$ac_includes_default" if test "x$ac_cv_have_decl_fwrite_unlocked" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_FWRITE_UNLOCKED $ac_have_decl _ACEOF ac_fn_c_check_decl "$LINENO" "getc_unlocked" "ac_cv_have_decl_getc_unlocked" "$ac_includes_default" if test "x$ac_cv_have_decl_getc_unlocked" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_GETC_UNLOCKED $ac_have_decl _ACEOF ac_fn_c_check_decl "$LINENO" "getchar_unlocked" "ac_cv_have_decl_getchar_unlocked" "$ac_includes_default" if test "x$ac_cv_have_decl_getchar_unlocked" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_GETCHAR_UNLOCKED $ac_have_decl _ACEOF ac_fn_c_check_decl "$LINENO" "putc_unlocked" "ac_cv_have_decl_putc_unlocked" "$ac_includes_default" if test "x$ac_cv_have_decl_putc_unlocked" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_PUTC_UNLOCKED $ac_have_decl _ACEOF ac_fn_c_check_decl "$LINENO" "putchar_unlocked" "ac_cv_have_decl_putchar_unlocked" "$ac_includes_default" if test "x$ac_cv_have_decl_putchar_unlocked" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_PUTCHAR_UNLOCKED $ac_have_decl _ACEOF for ac_func in $ac_func_list do : as_ac_var=`$as_echo "ac_cv_func_$ac_func" | $as_tr_sh` ac_fn_c_check_func "$LINENO" "$ac_func" "$as_ac_var" if eval test \"x\$"$as_ac_var"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_$ac_func" | $as_tr_cpp` 1 _ACEOF fi done for ac_header in $ac_header_list do : as_ac_Header=`$as_echo "ac_cv_header_$ac_header" | $as_tr_sh` ac_fn_c_check_header_compile "$LINENO" "$ac_header" "$as_ac_Header" "$ac_includes_default " if eval test \"x\$"$as_ac_Header"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_$ac_header" | $as_tr_cpp` 1 _ACEOF fi done ac_fn_c_check_decl "$LINENO" "strerror_r" "ac_cv_have_decl_strerror_r" "$ac_includes_default" if test "x$ac_cv_have_decl_strerror_r" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_STRERROR_R $ac_have_decl _ACEOF for ac_func in strerror_r do : ac_fn_c_check_func "$LINENO" "strerror_r" "ac_cv_func_strerror_r" if test "x$ac_cv_func_strerror_r" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STRERROR_R 1 _ACEOF fi done { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether strerror_r returns char *" >&5 $as_echo_n "checking whether strerror_r returns char *... 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" >&6; } if ${gl_cv_func_getopt_gnu+:} false; then : $as_echo_n "(cached) " >&6 else # Even with POSIXLY_CORRECT, the GNU extension of leading '-' in the # optstring is necessary for programs like m4 that have POSIX-mandated # semantics for supporting options interspersed with files. # Also, since getopt_long is a GNU extension, we require optind=0. # Bash ties 'set -o posix' to a non-exported POSIXLY_CORRECT; # so take care to revert to the correct (non-)export state. gl_awk_probe='BEGIN { if ("POSIXLY_CORRECT" in ENVIRON) print "x" }' case ${POSIXLY_CORRECT+x}`$AWK "$gl_awk_probe" conftest.$ac_ext /* end confdefs.h. */ #include #include #include #include #if defined __MACH__ && defined __APPLE__ /* Avoid a crash on Mac OS X. */ #include #include #include #include #include #include /* The exception port on which our thread listens. */ static mach_port_t our_exception_port; /* The main function of the thread listening for exceptions of type EXC_BAD_ACCESS. */ static void * mach_exception_thread (void *arg) { /* Buffer for a message to be received. */ struct { mach_msg_header_t head; mach_msg_body_t msgh_body; char data[1024]; } msg; mach_msg_return_t retval; /* Wait for a message on the exception port. */ retval = mach_msg (&msg.head, MACH_RCV_MSG | MACH_RCV_LARGE, 0, sizeof (msg), our_exception_port, MACH_MSG_TIMEOUT_NONE, MACH_PORT_NULL); if (retval != MACH_MSG_SUCCESS) abort (); exit (1); } static void nocrash_init (void) { mach_port_t self = mach_task_self (); /* Allocate a port on which the thread shall listen for exceptions. */ if (mach_port_allocate (self, MACH_PORT_RIGHT_RECEIVE, &our_exception_port) == KERN_SUCCESS) { /* See http://web.mit.edu/darwin/src/modules/xnu/osfmk/man/mach_port_insert_right.html. */ if (mach_port_insert_right (self, our_exception_port, our_exception_port, MACH_MSG_TYPE_MAKE_SEND) == KERN_SUCCESS) { /* The exceptions we want to catch. Only EXC_BAD_ACCESS is interesting for us. */ exception_mask_t mask = EXC_MASK_BAD_ACCESS; /* Create the thread listening on the exception port. */ pthread_attr_t attr; pthread_t thread; if (pthread_attr_init (&attr) == 0 && pthread_attr_setdetachstate (&attr, PTHREAD_CREATE_DETACHED) == 0 && pthread_create (&thread, &attr, mach_exception_thread, NULL) == 0) { pthread_attr_destroy (&attr); /* Replace the exception port info for these exceptions with our own. Note that we replace the exception port for the entire task, not only for a particular thread. This has the effect that when our exception port gets the message, the thread specific exception port has already been asked, and we don't need to bother about it. See http://web.mit.edu/darwin/src/modules/xnu/osfmk/man/task_set_exception_ports.html. */ task_set_exception_ports (self, mask, our_exception_port, EXCEPTION_DEFAULT, MACHINE_THREAD_STATE); } } } } #elif (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Avoid a crash on native Windows. */ #define WIN32_LEAN_AND_MEAN #include #include static LONG WINAPI exception_filter (EXCEPTION_POINTERS *ExceptionInfo) { switch (ExceptionInfo->ExceptionRecord->ExceptionCode) { case EXCEPTION_ACCESS_VIOLATION: case EXCEPTION_IN_PAGE_ERROR: case EXCEPTION_STACK_OVERFLOW: case EXCEPTION_GUARD_PAGE: case EXCEPTION_PRIV_INSTRUCTION: case EXCEPTION_ILLEGAL_INSTRUCTION: case EXCEPTION_DATATYPE_MISALIGNMENT: case EXCEPTION_ARRAY_BOUNDS_EXCEEDED: case EXCEPTION_NONCONTINUABLE_EXCEPTION: exit (1); } return EXCEPTION_CONTINUE_SEARCH; } static void nocrash_init (void) { SetUnhandledExceptionFilter ((LPTOP_LEVEL_EXCEPTION_FILTER) exception_filter); } #else /* Avoid a crash on POSIX systems. */ #include #include /* A POSIX signal handler. */ static void exception_handler (int sig) { _exit (1); } static void nocrash_init (void) { #ifdef SIGSEGV signal (SIGSEGV, exception_handler); #endif #ifdef SIGBUS signal (SIGBUS, exception_handler); #endif } #endif int main () { int result = 0; nocrash_init(); /* This code succeeds on glibc 2.8, OpenBSD 4.0, Cygwin, mingw, and fails on Mac OS X 10.5, AIX 5.2, HP-UX 11, IRIX 6.5, OSF/1 5.1, Solaris 10. */ { static char conftest[] = "conftest"; static char plus[] = "-+"; char *argv[3] = { conftest, plus, NULL }; opterr = 0; if (getopt (2, argv, "+a") != '?') result |= 1; } /* This code succeeds on glibc 2.8, mingw, and fails on Mac OS X 10.5, OpenBSD 4.0, AIX 5.2, HP-UX 11, IRIX 6.5, OSF/1 5.1, Solaris 10, Cygwin 1.5.x. */ { static char program[] = "program"; static char p[] = "-p"; static char foo[] = "foo"; static char bar[] = "bar"; char *argv[] = { program, p, foo, bar, NULL }; optind = 1; if (getopt (4, argv, "p::") != 'p') result |= 2; else if (optarg != NULL) result |= 4; else if (getopt (4, argv, "p::") != -1) result |= 6; else if (optind != 2) result |= 8; } /* This code succeeds on glibc 2.8 and fails on Cygwin 1.7.0. */ { static char program[] = "program"; static char foo[] = "foo"; static char p[] = "-p"; char *argv[] = { program, foo, p, NULL }; optind = 0; if (getopt (3, argv, "-p") != 1) result |= 16; else if (getopt (3, argv, "-p") != 'p') result |= 16; } /* This code fails on glibc 2.11. */ { static char program[] = "program"; static char b[] = "-b"; static char a[] = "-a"; char *argv[] = { program, b, a, NULL }; optind = opterr = 0; if (getopt (3, argv, "+:a:b") != 'b') result |= 32; else if (getopt (3, argv, "+:a:b") != ':') result |= 32; } /* This code dumps core on glibc 2.14. */ { static char program[] = "program"; static char w[] = "-W"; static char dummy[] = "dummy"; char *argv[] = { program, w, dummy, NULL }; optind = opterr = 1; if (getopt (3, argv, "W;") != 'W') result |= 64; } return result; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_getopt_gnu=yes else gl_cv_func_getopt_gnu=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi case $gl_had_POSIXLY_CORRECT in exported) ;; yes) { POSIXLY_CORRECT=; unset POSIXLY_CORRECT;}; POSIXLY_CORRECT=1 ;; *) { POSIXLY_CORRECT=; unset POSIXLY_CORRECT;} ;; esac fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_getopt_gnu" >&5 $as_echo "$gl_cv_func_getopt_gnu" >&6; } if test "$gl_cv_func_getopt_gnu" != yes; then gl_replace_getopt=yes else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for working GNU getopt_long function" >&5 $as_echo_n "checking for working GNU getopt_long function... " >&6; } if ${gl_cv_func_getopt_long_gnu+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in openbsd*) gl_cv_func_getopt_long_gnu="guessing no";; *) gl_cv_func_getopt_long_gnu="guessing yes";; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include int main () { static const struct option long_options[] = { { "xtremely-",no_argument, NULL, 1003 }, { "xtra", no_argument, NULL, 1001 }, { "xtreme", no_argument, NULL, 1002 }, { "xtremely", no_argument, NULL, 1003 }, { NULL, 0, NULL, 0 } }; /* This code fails on OpenBSD 5.0. */ { static char program[] = "program"; static char xtremel[] = "--xtremel"; char *argv[] = { program, xtremel, NULL }; int option_index; optind = 1; opterr = 0; if (getopt_long (2, argv, "", long_options, &option_index) != 1003) return 1; } return 0; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_getopt_long_gnu=yes else gl_cv_func_getopt_long_gnu=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_getopt_long_gnu" >&5 $as_echo "$gl_cv_func_getopt_long_gnu" >&6; } case "$gl_cv_func_getopt_long_gnu" in *yes) ;; *) gl_replace_getopt=yes ;; esac fi fi REPLACE_GETOPT=1 if test $REPLACE_GETOPT = 1; then GETOPT_H=getopt.h $as_echo "#define __GETOPT_PREFIX rpl_" >>confdefs.h fi ac_fn_c_check_decl "$LINENO" "getenv" "ac_cv_have_decl_getenv" "$ac_includes_default" if test "x$ac_cv_have_decl_getenv" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_GETENV $ac_have_decl _ACEOF GNULIB_NL_LANGINFO=0; HAVE_NL_LANGINFO=1; REPLACE_NL_LANGINFO=0; if test $gl_cv_have_include_next = yes; then gl_cv_next_limits_h='<'limits.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_limits_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_limits_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'limits.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_limits_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_limits_h gl_cv_next_limits_h='"'$gl_header'"' else gl_cv_next_limits_h='<'limits.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_limits_h" >&5 $as_echo "$gl_cv_next_limits_h" >&6; } fi NEXT_LIMITS_H=$gl_cv_next_limits_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'limits.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_limits_h fi NEXT_AS_FIRST_DIRECTIVE_LIMITS_H=$gl_next_as_first_directive { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether limits.h has ULLONG_WIDTH etc." >&5 $as_echo_n "checking whether limits.h has ULLONG_WIDTH etc.... 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Note that ksh looks also at the FPATH variable, # so we have to set that as well for the test. PATH_SEPARATOR=: (PATH='/bin;/bin'; FPATH=$PATH; sh -c :) >/dev/null 2>&1 \ && { (PATH='/bin:/bin'; FPATH=$PATH; sh -c :) >/dev/null 2>&1 \ || PATH_SEPARATOR=';' } fi ac_prog=ld if test "$GCC" = yes; then # Check if gcc -print-prog-name=ld gives a path. { $as_echo "$as_me:${as_lineno-$LINENO}: checking for ld used by $CC" >&5 $as_echo_n "checking for ld used by $CC... " >&6; } case $host in *-*-mingw*) # gcc leaves a trailing carriage return which upsets mingw ac_prog=`($CC -print-prog-name=ld) 2>&5 | tr -d '\015'` ;; *) ac_prog=`($CC -print-prog-name=ld) 2>&5` ;; esac case $ac_prog in # Accept absolute paths. [\\/]* | ?:[\\/]*) re_direlt='/[^/][^/]*/\.\./' # Canonicalize the pathname of ld ac_prog=`echo "$ac_prog"| sed 's%\\\\%/%g'` while echo "$ac_prog" | grep "$re_direlt" > /dev/null 2>&1; do ac_prog=`echo $ac_prog| sed "s%$re_direlt%/%"` done test -z "$LD" && LD="$ac_prog" ;; "") # If it fails, then pretend we aren't using GCC. ac_prog=ld ;; *) # If it is relative, then search for the first ld in PATH. with_gnu_ld=unknown ;; esac elif test "$with_gnu_ld" = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking for GNU ld" >&5 $as_echo_n "checking for GNU ld... " >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for non-GNU ld" >&5 $as_echo_n "checking for non-GNU ld... " >&6; } fi if ${acl_cv_path_LD+:} false; then : $as_echo_n "(cached) " >&6 else if test -z "$LD"; then acl_save_ifs="$IFS"; IFS=$PATH_SEPARATOR for ac_dir in $PATH; do IFS="$acl_save_ifs" test -z "$ac_dir" && ac_dir=. if test -f "$ac_dir/$ac_prog" || test -f "$ac_dir/$ac_prog$ac_exeext"; then acl_cv_path_LD="$ac_dir/$ac_prog" # Check to see if the program is GNU ld. I'd rather use --version, # but apparently some variants of GNU ld only accept -v. # Break only if it was the GNU/non-GNU ld that we prefer. case `"$acl_cv_path_LD" -v 2>&1 &5 $as_echo "$LD" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi test -z "$LD" && as_fn_error $? "no acceptable ld found in \$PATH" "$LINENO" 5 { $as_echo "$as_me:${as_lineno-$LINENO}: checking if the linker ($LD) is GNU ld" >&5 $as_echo_n "checking if the linker ($LD) is GNU ld... 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" >&6; } if ${gl_cv_solaris_64bit+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifdef _LP64 sixtyfour bits #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "sixtyfour bits" >/dev/null 2>&1; then : gl_cv_solaris_64bit=yes else gl_cv_solaris_64bit=no fi rm -f conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_solaris_64bit" >&5 $as_echo "$gl_cv_solaris_64bit" >&6; } if test $gl_cv_solaris_64bit = yes; then acl_libdirstem=lib/64 case "$host_cpu" in sparc*) acl_libdirstem2=lib/sparcv9 ;; i*86 | x86_64) acl_libdirstem2=lib/amd64 ;; esac fi ;; *) searchpath=`(LC_ALL=C $CC -print-search-dirs) 2>/dev/null | sed -n -e 's,^libraries: ,,p' | sed -e 's,^=,,'` if test -n "$searchpath"; then acl_save_IFS="${IFS= }"; IFS=":" for searchdir in $searchpath; do if test -d "$searchdir"; then case "$searchdir" in */lib64/ | */lib64 ) acl_libdirstem=lib64 ;; */../ | */.. ) # Better ignore directories of this form. They are misleading. ;; *) searchdir=`cd "$searchdir" && pwd` case "$searchdir" in */lib64 ) acl_libdirstem=lib64 ;; esac ;; esac fi done IFS="$acl_save_IFS" fi ;; esac test -n "$acl_libdirstem2" || acl_libdirstem2="$acl_libdirstem" gl_threads_api=none LIBTHREAD= LTLIBTHREAD= LIBMULTITHREAD= LTLIBMULTITHREAD= if test "$gl_use_threads" != no; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether imported symbols can be declared weak" >&5 $as_echo_n "checking whether imported symbols can be declared weak... " >&6; } if ${gl_cv_have_weak+:} false; then : $as_echo_n "(cached) " >&6 else gl_cv_have_weak=no cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ extern void xyzzy (); #pragma weak xyzzy int main () { xyzzy(); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_cv_have_weak=maybe fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext if test $gl_cv_have_weak = maybe; then if test "$cross_compiling" = yes; then : cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifdef __ELF__ Extensible Linking Format #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "Extensible Linking Format" >/dev/null 2>&1; then : gl_cv_have_weak="guessing yes" else gl_cv_have_weak="guessing no" fi rm -f conftest* else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #pragma weak fputs int main () { return (fputs == NULL); } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_have_weak=yes else gl_cv_have_weak=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_have_weak" >&5 $as_echo "$gl_cv_have_weak" >&6; } if test "$gl_use_threads" = yes || test "$gl_use_threads" = posix; then # On OSF/1, the compiler needs the flag -pthread or -D_REENTRANT so that # it groks . It's added above, in gl_THREADLIB_EARLY_BODY. ac_fn_c_check_header_mongrel "$LINENO" "pthread.h" "ac_cv_header_pthread_h" "$ac_includes_default" if test "x$ac_cv_header_pthread_h" = xyes; then : gl_have_pthread_h=yes else gl_have_pthread_h=no fi if test "$gl_have_pthread_h" = yes; then # Other possible tests: # -lpthreads (FSU threads, PCthreads) # -lgthreads gl_have_pthread= # Test whether both pthread_mutex_lock and pthread_mutexattr_init exist # in libc. IRIX 6.5 has the first one in both libc and libpthread, but # the second one only in libpthread, and lock.c needs it. # # If -pthread works, prefer it to -lpthread, since Ubuntu 14.04 # needs -pthread for some reason. See: # http://lists.gnu.org/archive/html/bug-gnulib/2014-09/msg00023.html save_LIBS=$LIBS for gl_pthread in '' '-pthread'; do LIBS="$LIBS $gl_pthread" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include pthread_mutex_t m; pthread_mutexattr_t ma; int main () { pthread_mutex_lock (&m); pthread_mutexattr_init (&ma); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_have_pthread=yes LIBTHREAD=$gl_pthread LTLIBTHREAD=$gl_pthread LIBMULTITHREAD=$gl_pthread LTLIBMULTITHREAD=$gl_pthread fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS=$save_LIBS test -n "$gl_have_pthread" && break done # Test for libpthread by looking for pthread_kill. (Not pthread_self, # since it is defined as a macro on OSF/1.) if test -n "$gl_have_pthread" && test -z "$LIBTHREAD"; then # The program links fine without libpthread. But it may actually # need to link with libpthread in order to create multiple threads. { $as_echo "$as_me:${as_lineno-$LINENO}: checking for pthread_kill in -lpthread" >&5 $as_echo_n "checking for pthread_kill in -lpthread... " >&6; } if ${ac_cv_lib_pthread_pthread_kill+:} false; then : $as_echo_n "(cached) " >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lpthread $LIBS" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char pthread_kill (); int main () { return pthread_kill (); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : ac_cv_lib_pthread_pthread_kill=yes else ac_cv_lib_pthread_pthread_kill=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_lib_pthread_pthread_kill" >&5 $as_echo "$ac_cv_lib_pthread_pthread_kill" >&6; } if test "x$ac_cv_lib_pthread_pthread_kill" = xyes; then : LIBMULTITHREAD=-lpthread LTLIBMULTITHREAD=-lpthread # On Solaris and HP-UX, most pthread functions exist also in libc. # Therefore pthread_in_use() needs to actually try to create a # thread: pthread_create from libc will fail, whereas # pthread_create will actually create a thread. case "$host_os" in solaris* | hpux*) $as_echo "#define PTHREAD_IN_USE_DETECTION_HARD 1" >>confdefs.h esac fi elif test -z "$gl_have_pthread"; then # Some library is needed. Try libpthread and libc_r. { $as_echo "$as_me:${as_lineno-$LINENO}: checking for pthread_kill in -lpthread" >&5 $as_echo_n "checking for pthread_kill in -lpthread... " >&6; } if ${ac_cv_lib_pthread_pthread_kill+:} false; then : $as_echo_n "(cached) " >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lpthread $LIBS" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char pthread_kill (); int main () { return pthread_kill (); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : ac_cv_lib_pthread_pthread_kill=yes else ac_cv_lib_pthread_pthread_kill=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_lib_pthread_pthread_kill" >&5 $as_echo "$ac_cv_lib_pthread_pthread_kill" >&6; } if test "x$ac_cv_lib_pthread_pthread_kill" = xyes; then : gl_have_pthread=yes LIBTHREAD=-lpthread LTLIBTHREAD=-lpthread LIBMULTITHREAD=-lpthread LTLIBMULTITHREAD=-lpthread fi if test -z "$gl_have_pthread"; then # For FreeBSD 4. { $as_echo "$as_me:${as_lineno-$LINENO}: checking for pthread_kill in -lc_r" >&5 $as_echo_n "checking for pthread_kill in -lc_r... 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Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char pthread_kill (); int main () { return pthread_kill (); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : ac_cv_lib_c_r_pthread_kill=yes else ac_cv_lib_c_r_pthread_kill=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_lib_c_r_pthread_kill" >&5 $as_echo "$ac_cv_lib_c_r_pthread_kill" >&6; } if test "x$ac_cv_lib_c_r_pthread_kill" = xyes; then : gl_have_pthread=yes LIBTHREAD=-lc_r LTLIBTHREAD=-lc_r LIBMULTITHREAD=-lc_r LTLIBMULTITHREAD=-lc_r fi fi fi if test -n "$gl_have_pthread"; then gl_threads_api=posix $as_echo "#define USE_POSIX_THREADS 1" >>confdefs.h if test -n "$LIBMULTITHREAD" || test -n "$LTLIBMULTITHREAD"; then if case "$gl_cv_have_weak" in *yes) true;; *) false;; esac; then $as_echo "#define USE_POSIX_THREADS_WEAK 1" >>confdefs.h LIBTHREAD= LTLIBTHREAD= fi fi fi fi fi if test -z "$gl_have_pthread"; then if test "$gl_use_threads" = yes || test "$gl_use_threads" = solaris; then gl_have_solaristhread= gl_save_LIBS="$LIBS" LIBS="$LIBS -lthread" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int main () { thr_self(); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_have_solaristhread=yes fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS="$gl_save_LIBS" if test -n "$gl_have_solaristhread"; then gl_threads_api=solaris LIBTHREAD=-lthread LTLIBTHREAD=-lthread LIBMULTITHREAD="$LIBTHREAD" LTLIBMULTITHREAD="$LTLIBTHREAD" $as_echo "#define USE_SOLARIS_THREADS 1" >>confdefs.h if case "$gl_cv_have_weak" in *yes) true;; *) false;; esac; then $as_echo "#define USE_SOLARIS_THREADS_WEAK 1" >>confdefs.h LIBTHREAD= LTLIBTHREAD= fi fi fi fi if test "$gl_use_threads" = pth; then gl_save_CPPFLAGS="$CPPFLAGS" { $as_echo "$as_me:${as_lineno-$LINENO}: checking how to link with libpth" >&5 $as_echo_n "checking how to link with libpth... " >&6; } if ${ac_cv_libpth_libs+:} false; then : $as_echo_n "(cached) " >&6 else use_additional=yes acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" eval additional_includedir=\"$includedir\" eval additional_libdir=\"$libdir\" exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" # Check whether --with-libpth-prefix was given. if test "${with_libpth_prefix+set}" = set; then : withval=$with_libpth_prefix; if test "X$withval" = "Xno"; then use_additional=no else if test "X$withval" = "X"; then acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" eval additional_includedir=\"$includedir\" eval additional_libdir=\"$libdir\" exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" else additional_includedir="$withval/include" additional_libdir="$withval/$acl_libdirstem" if test "$acl_libdirstem2" != "$acl_libdirstem" \ && ! test -d "$withval/$acl_libdirstem"; then additional_libdir="$withval/$acl_libdirstem2" fi fi fi fi LIBPTH= LTLIBPTH= INCPTH= LIBPTH_PREFIX= HAVE_LIBPTH= rpathdirs= ltrpathdirs= names_already_handled= names_next_round='pth ' while test -n "$names_next_round"; do names_this_round="$names_next_round" names_next_round= for name in $names_this_round; do already_handled= for n in $names_already_handled; do if test "$n" = "$name"; then already_handled=yes break fi done if test -z "$already_handled"; then names_already_handled="$names_already_handled $name" uppername=`echo "$name" | sed -e 'y|abcdefghijklmnopqrstuvwxyz./+-|ABCDEFGHIJKLMNOPQRSTUVWXYZ____|'` eval value=\"\$HAVE_LIB$uppername\" if test -n "$value"; then if test "$value" = yes; then eval value=\"\$LIB$uppername\" test -z "$value" || LIBPTH="${LIBPTH}${LIBPTH:+ }$value" eval value=\"\$LTLIB$uppername\" test -z "$value" || LTLIBPTH="${LTLIBPTH}${LTLIBPTH:+ }$value" else : fi else found_dir= found_la= found_so= found_a= eval libname=\"$acl_libname_spec\" # typically: libname=lib$name if test -n "$acl_shlibext"; then shrext=".$acl_shlibext" # typically: shrext=.so else shrext= fi if test $use_additional = yes; then dir="$additional_libdir" if test -n "$acl_shlibext"; then if test -f "$dir/$libname$shrext"; then found_dir="$dir" found_so="$dir/$libname$shrext" else if test "$acl_library_names_spec" = '$libname$shrext$versuffix'; then ver=`(cd "$dir" && \ for f in "$libname$shrext".*; do echo "$f"; done \ | sed -e "s,^$libname$shrext\\\\.,," \ | sort -t '.' -n -r -k1,1 -k2,2 -k3,3 -k4,4 -k5,5 \ | sed 1q ) 2>/dev/null` if test -n "$ver" && test -f "$dir/$libname$shrext.$ver"; then found_dir="$dir" found_so="$dir/$libname$shrext.$ver" fi else eval library_names=\"$acl_library_names_spec\" for f in $library_names; do if test -f "$dir/$f"; then found_dir="$dir" found_so="$dir/$f" break fi done fi fi fi if test "X$found_dir" = "X"; then if test -f "$dir/$libname.$acl_libext"; then found_dir="$dir" found_a="$dir/$libname.$acl_libext" fi fi if test "X$found_dir" != "X"; then if test -f "$dir/$libname.la"; then found_la="$dir/$libname.la" fi fi fi if test "X$found_dir" = "X"; then for x in $LDFLAGS $LTLIBPTH; do acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" eval x=\"$x\" exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" case "$x" in -L*) dir=`echo "X$x" | sed -e 's/^X-L//'` if test -n "$acl_shlibext"; then if test -f "$dir/$libname$shrext"; then found_dir="$dir" found_so="$dir/$libname$shrext" else if test "$acl_library_names_spec" = '$libname$shrext$versuffix'; then ver=`(cd "$dir" && \ for f in "$libname$shrext".*; do echo "$f"; done \ | sed -e "s,^$libname$shrext\\\\.,," \ | sort -t '.' -n -r -k1,1 -k2,2 -k3,3 -k4,4 -k5,5 \ | sed 1q ) 2>/dev/null` if test -n "$ver" && test -f "$dir/$libname$shrext.$ver"; then found_dir="$dir" found_so="$dir/$libname$shrext.$ver" fi else eval library_names=\"$acl_library_names_spec\" for f in $library_names; do if test -f "$dir/$f"; then found_dir="$dir" found_so="$dir/$f" break fi done fi fi fi if test "X$found_dir" = "X"; then if test -f "$dir/$libname.$acl_libext"; then found_dir="$dir" found_a="$dir/$libname.$acl_libext" fi fi if test "X$found_dir" != "X"; then if test -f "$dir/$libname.la"; then found_la="$dir/$libname.la" fi fi ;; esac if test "X$found_dir" != "X"; then break fi done fi if test "X$found_dir" != "X"; then LTLIBPTH="${LTLIBPTH}${LTLIBPTH:+ }-L$found_dir -l$name" if test "X$found_so" != "X"; then if test "$enable_rpath" = no \ || test "X$found_dir" = "X/usr/$acl_libdirstem" \ || test "X$found_dir" = "X/usr/$acl_libdirstem2"; then LIBPTH="${LIBPTH}${LIBPTH:+ }$found_so" else haveit= for x in $ltrpathdirs; do if test "X$x" = "X$found_dir"; then haveit=yes break fi done if test -z "$haveit"; then ltrpathdirs="$ltrpathdirs $found_dir" fi if test "$acl_hardcode_direct" = yes; then LIBPTH="${LIBPTH}${LIBPTH:+ }$found_so" else if test -n "$acl_hardcode_libdir_flag_spec" && test "$acl_hardcode_minus_L" = no; then LIBPTH="${LIBPTH}${LIBPTH:+ }$found_so" haveit= for x in $rpathdirs; do if test "X$x" = "X$found_dir"; then haveit=yes break fi done if test -z "$haveit"; then rpathdirs="$rpathdirs $found_dir" fi else haveit= for x in $LDFLAGS $LIBPTH; do acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" eval x=\"$x\" exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" if test "X$x" = "X-L$found_dir"; then haveit=yes break fi done if test -z "$haveit"; then LIBPTH="${LIBPTH}${LIBPTH:+ }-L$found_dir" fi if test "$acl_hardcode_minus_L" != no; then LIBPTH="${LIBPTH}${LIBPTH:+ }$found_so" else LIBPTH="${LIBPTH}${LIBPTH:+ }-l$name" fi fi fi fi else if test "X$found_a" != "X"; then LIBPTH="${LIBPTH}${LIBPTH:+ }$found_a" else LIBPTH="${LIBPTH}${LIBPTH:+ }-L$found_dir -l$name" fi fi additional_includedir= case "$found_dir" in */$acl_libdirstem | */$acl_libdirstem/) basedir=`echo "X$found_dir" | sed -e 's,^X,,' -e "s,/$acl_libdirstem/"'*$,,'` if test "$name" = 'pth'; then LIBPTH_PREFIX="$basedir" fi additional_includedir="$basedir/include" ;; */$acl_libdirstem2 | */$acl_libdirstem2/) basedir=`echo "X$found_dir" | sed -e 's,^X,,' -e "s,/$acl_libdirstem2/"'*$,,'` if test "$name" = 'pth'; then LIBPTH_PREFIX="$basedir" fi additional_includedir="$basedir/include" ;; esac if test "X$additional_includedir" != "X"; then if test "X$additional_includedir" != "X/usr/include"; then haveit= if test "X$additional_includedir" = "X/usr/local/include"; then if test -n "$GCC"; then case $host_os in linux* | gnu* | k*bsd*-gnu) haveit=yes;; esac fi fi if test -z "$haveit"; then for x in $CPPFLAGS $INCPTH; do acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" eval x=\"$x\" exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" if test "X$x" = "X-I$additional_includedir"; then haveit=yes break fi done if test -z "$haveit"; then if test -d "$additional_includedir"; then INCPTH="${INCPTH}${INCPTH:+ }-I$additional_includedir" fi fi fi fi fi if test -n "$found_la"; then save_libdir="$libdir" case "$found_la" in */* | *\\*) . "$found_la" ;; *) . "./$found_la" ;; esac libdir="$save_libdir" for dep in $dependency_libs; do case "$dep" in -L*) additional_libdir=`echo "X$dep" | sed -e 's/^X-L//'` if test "X$additional_libdir" != "X/usr/$acl_libdirstem" \ && test "X$additional_libdir" != "X/usr/$acl_libdirstem2"; then haveit= if test "X$additional_libdir" = "X/usr/local/$acl_libdirstem" \ || test "X$additional_libdir" = "X/usr/local/$acl_libdirstem2"; then if test -n "$GCC"; then case $host_os in linux* | gnu* | k*bsd*-gnu) haveit=yes;; esac fi fi if test -z "$haveit"; then haveit= for x in $LDFLAGS $LIBPTH; do acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" eval x=\"$x\" exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" if test "X$x" = "X-L$additional_libdir"; then haveit=yes break fi done if test -z "$haveit"; then if test -d "$additional_libdir"; then LIBPTH="${LIBPTH}${LIBPTH:+ }-L$additional_libdir" fi fi haveit= for x in $LDFLAGS $LTLIBPTH; do acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" eval x=\"$x\" exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" if test "X$x" = "X-L$additional_libdir"; then haveit=yes break fi done if test -z "$haveit"; then if test -d "$additional_libdir"; then LTLIBPTH="${LTLIBPTH}${LTLIBPTH:+ }-L$additional_libdir" fi fi fi fi ;; -R*) dir=`echo "X$dep" | sed -e 's/^X-R//'` if test "$enable_rpath" != no; then haveit= for x in $rpathdirs; do if test "X$x" = "X$dir"; then haveit=yes break fi done if test -z "$haveit"; then rpathdirs="$rpathdirs $dir" fi haveit= for x in $ltrpathdirs; do if test "X$x" = "X$dir"; then haveit=yes break fi done if test -z "$haveit"; then ltrpathdirs="$ltrpathdirs $dir" fi fi ;; -l*) names_next_round="$names_next_round "`echo "X$dep" | sed -e 's/^X-l//'` ;; *.la) names_next_round="$names_next_round "`echo "X$dep" | sed -e 's,^X.*/,,' -e 's,^lib,,' -e 's,\.la$,,'` ;; *) LIBPTH="${LIBPTH}${LIBPTH:+ }$dep" LTLIBPTH="${LTLIBPTH}${LTLIBPTH:+ }$dep" ;; esac done fi else LIBPTH="${LIBPTH}${LIBPTH:+ }-l$name" LTLIBPTH="${LTLIBPTH}${LTLIBPTH:+ }-l$name" fi fi fi done done if test "X$rpathdirs" != "X"; then if test -n "$acl_hardcode_libdir_separator"; then alldirs= for found_dir in $rpathdirs; do alldirs="${alldirs}${alldirs:+$acl_hardcode_libdir_separator}$found_dir" done acl_save_libdir="$libdir" libdir="$alldirs" eval flag=\"$acl_hardcode_libdir_flag_spec\" libdir="$acl_save_libdir" LIBPTH="${LIBPTH}${LIBPTH:+ }$flag" else for found_dir in $rpathdirs; do acl_save_libdir="$libdir" libdir="$found_dir" eval flag=\"$acl_hardcode_libdir_flag_spec\" libdir="$acl_save_libdir" LIBPTH="${LIBPTH}${LIBPTH:+ }$flag" done fi fi if test "X$ltrpathdirs" != "X"; then for found_dir in $ltrpathdirs; do LTLIBPTH="${LTLIBPTH}${LTLIBPTH:+ }-R$found_dir" done fi ac_cv_libpth_libs="$LIBPTH" ac_cv_libpth_ltlibs="$LTLIBPTH" ac_cv_libpth_cppflags="$INCPTH" ac_cv_libpth_prefix="$LIBPTH_PREFIX" fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_libpth_libs" >&5 $as_echo "$ac_cv_libpth_libs" >&6; } LIBPTH="$ac_cv_libpth_libs" LTLIBPTH="$ac_cv_libpth_ltlibs" INCPTH="$ac_cv_libpth_cppflags" LIBPTH_PREFIX="$ac_cv_libpth_prefix" for element in $INCPTH; do haveit= for x in $CPPFLAGS; do acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" eval x=\"$x\" exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" if test "X$x" = "X$element"; then haveit=yes break fi done if test -z "$haveit"; then CPPFLAGS="${CPPFLAGS}${CPPFLAGS:+ }$element" fi done HAVE_LIBPTH=yes gl_have_pth= gl_save_LIBS="$LIBS" LIBS="$LIBS $LIBPTH" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { pth_self(); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_have_pth=yes fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS="$gl_save_LIBS" if test -n "$gl_have_pth"; then gl_threads_api=pth LIBTHREAD="$LIBPTH" LTLIBTHREAD="$LTLIBPTH" LIBMULTITHREAD="$LIBTHREAD" LTLIBMULTITHREAD="$LTLIBTHREAD" $as_echo "#define USE_PTH_THREADS 1" >>confdefs.h if test -n "$LIBMULTITHREAD" || test -n "$LTLIBMULTITHREAD"; then if case "$gl_cv_have_weak" in *yes) true;; *) false;; esac; then $as_echo "#define USE_PTH_THREADS_WEAK 1" >>confdefs.h LIBTHREAD= LTLIBTHREAD= fi fi else CPPFLAGS="$gl_save_CPPFLAGS" fi fi if test -z "$gl_have_pthread"; then case "$gl_use_threads" in yes | windows | win32) # The 'win32' is for backward compatibility. if { case "$host_os" in mingw*) true;; *) false;; esac }; then gl_threads_api=windows $as_echo "#define USE_WINDOWS_THREADS 1" >>confdefs.h fi ;; esac fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for multithread API to use" >&5 $as_echo_n "checking for multithread API to use... 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" >&6; } if ${ac_cv_type_mbstate_t+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ $ac_includes_default /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { mbstate_t x; return sizeof x; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_type_mbstate_t=yes else ac_cv_type_mbstate_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_type_mbstate_t" >&5 $as_echo "$ac_cv_type_mbstate_t" >&6; } if test $ac_cv_type_mbstate_t = yes; then $as_echo "#define HAVE_MBSTATE_T 1" >>confdefs.h else $as_echo "#define mbstate_t int" >>confdefs.h fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a traditional japanese locale" >&5 $as_echo_n "checking for a traditional japanese locale... " >&6; } if ${gt_cv_locale_ja+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { const char *p; /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether MB_CUR_MAX is > 1. This excludes the dysfunctional locales on Cygwin 1.5.x. */ if (MB_CUR_MAX == 1) return 1; /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Note that on native Windows, the Japanese locale is # Japanese_Japan.932, and CP932 is very different from EUC-JP, so we # cannot use it here. gt_cv_locale_ja=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the AIX locale name. if (LC_ALL=ja_JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP else # Test for the locale name with explicit encoding suffix. if (LC_ALL=ja_JP.EUC-JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC-JP else # Test for the HP-UX, OSF/1, NetBSD locale name. if (LC_ALL=ja_JP.eucJP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.eucJP else # Test for the IRIX, FreeBSD locale name. if (LC_ALL=ja_JP.EUC LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC else # Test for the Solaris 7 locale name. if (LC_ALL=ja LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja else # Special test for NetBSD 1.6. if test -f /usr/share/locale/ja_JP.eucJP/LC_CTYPE; then gt_cv_locale_ja=ja_JP.eucJP else # None found. gt_cv_locale_ja=none fi fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_ja" >&5 $as_echo "$gt_cv_locale_ja" >&6; } LOCALE_JA=$gt_cv_locale_ja { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a transitional chinese locale" >&5 $as_echo_n "checking for a transitional chinese locale... " >&6; } if ${gt_cv_locale_zh_CN+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { const char *p; /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; /* Check whether a typical GB18030 multibyte sequence is recognized as a single wide character. This excludes the GB2312 and GBK encodings. */ if (mblen ("\203\062\332\066", 5) != 4) return 1; return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=Chinese_China.54936 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=Chinese_China.54936 else # None found. gt_cv_locale_zh_CN=none fi ;; solaris2.8) # On Solaris 8, the locales zh_CN.GB18030, zh_CN.GBK, zh.GBK are # broken. One witness is the test case in gl_MBRTOWC_SANITYCHECK. # Another witness is that "LC_ALL=zh_CN.GB18030 bash -c true" dumps core. gt_cv_locale_zh_CN=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the locale name without encoding suffix. if (LC_ALL=zh_CN LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN else # Test for the locale name with explicit encoding suffix. if (LC_ALL=zh_CN.GB18030 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN.GB18030 else # None found. gt_cv_locale_zh_CN=none fi fi ;; esac else # If there was a link error, due to mblen(), the system is so old that # it certainly doesn't have a chinese locale. gt_cv_locale_zh_CN=none fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_zh_CN" >&5 $as_echo "$gt_cv_locale_zh_CN" >&6; } LOCALE_ZH_CN=$gt_cv_locale_zh_CN { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a french Unicode locale" >&5 $as_echo_n "checking for a french Unicode locale... 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In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. 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Don't use AC_FUNC_MMAP, because it checks too much: it # fails on HP-UX 11, because MAP_FIXED mappings do not work. But this is # irrelevant for anonymous mappings. ac_fn_c_check_func "$LINENO" "mmap" "ac_cv_func_mmap" if test "x$ac_cv_func_mmap" = xyes; then : gl_have_mmap=yes else gl_have_mmap=no fi # Try to allow MAP_ANONYMOUS. gl_have_mmap_anonymous=no if test $gl_have_mmap = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking for MAP_ANONYMOUS" >&5 $as_echo_n "checking for MAP_ANONYMOUS... 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" >&6; } if ${gl_cv_func_memchr_works+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : gl_cv_func_memchr_works="guessing no" else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #if HAVE_SYS_MMAN_H # include # include # include # include # ifndef MAP_FILE # define MAP_FILE 0 # endif #endif int main () { int result = 0; char *fence = NULL; #if HAVE_SYS_MMAN_H && HAVE_MPROTECT # if HAVE_MAP_ANONYMOUS const int flags = MAP_ANONYMOUS | MAP_PRIVATE; const int fd = -1; # else /* !HAVE_MAP_ANONYMOUS */ const int flags = MAP_FILE | MAP_PRIVATE; int fd = open ("/dev/zero", O_RDONLY, 0666); if (fd >= 0) # endif { int pagesize = getpagesize (); char *two_pages = (char *) mmap (NULL, 2 * pagesize, PROT_READ | PROT_WRITE, flags, fd, 0); if (two_pages != (char *)(-1) && mprotect (two_pages + pagesize, pagesize, PROT_NONE) == 0) fence = two_pages + pagesize; } #endif if (fence) { if (memchr (fence, 0, 0)) result |= 1; strcpy (fence - 9, "12345678"); if (memchr (fence - 9, 0, 79) != fence - 1) result |= 2; if (memchr (fence - 1, 0, 3) != fence - 1) result |= 4; } return result; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_memchr_works=yes else gl_cv_func_memchr_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_memchr_works" >&5 $as_echo "$gl_cv_func_memchr_works" >&6; } if test "$gl_cv_func_memchr_works" != yes; then REPLACE_MEMCHR=1 fi fi if test $ac_cv_func__set_invalid_parameter_handler = yes; then HAVE_MSVC_INVALID_PARAMETER_HANDLER=1 $as_echo "#define HAVE_MSVC_INVALID_PARAMETER_HANDLER 1" >>confdefs.h else HAVE_MSVC_INVALID_PARAMETER_HANDLER=0 fi gl_cv_c_multiarch=no cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifndef __APPLE_CC__ not a universal capable compiler #endif typedef int dummy; _ACEOF if ac_fn_c_try_compile "$LINENO"; then : arch= prev= for word in ${CC} ${CFLAGS} ${CPPFLAGS} ${LDFLAGS}; do if test -n "$prev"; then case $word in i?86 | x86_64 | ppc | ppc64) if test -z "$arch" || test "$arch" = "$word"; then arch="$word" else gl_cv_c_multiarch=yes fi ;; esac prev= else if test "x$word" = "x-arch"; then prev=arch fi fi done fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext if test $gl_cv_c_multiarch = yes; then APPLE_UNIVERSAL_BUILD=1 else APPLE_UNIVERSAL_BUILD=0 fi ac_fn_c_check_decl "$LINENO" "alarm" "ac_cv_have_decl_alarm" "$ac_includes_default" if test "x$ac_cv_have_decl_alarm" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_ALARM $ac_have_decl _ACEOF for ac_header in stdlib.h do : ac_fn_c_check_header_mongrel "$LINENO" "stdlib.h" "ac_cv_header_stdlib_h" "$ac_includes_default" if test "x$ac_cv_header_stdlib_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STDLIB_H 1 _ACEOF fi done { $as_echo "$as_me:${as_lineno-$LINENO}: checking for GNU libc compatible malloc" >&5 $as_echo_n "checking for GNU libc compatible malloc... " >&6; } if ${ac_cv_func_malloc_0_nonnull+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on platforms where we know the result. *-gnu* | freebsd* | netbsd* | openbsd* \ | hpux* | solaris* | cygwin* | mingw*) ac_cv_func_malloc_0_nonnull=yes ;; # If we don't know, assume the worst. *) ac_cv_func_malloc_0_nonnull=no ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if defined STDC_HEADERS || defined HAVE_STDLIB_H # include #else char *malloc (); #endif int main () { char *p = malloc (0); int result = !p; free (p); return result; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : ac_cv_func_malloc_0_nonnull=yes else ac_cv_func_malloc_0_nonnull=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_func_malloc_0_nonnull" >&5 $as_echo "$ac_cv_func_malloc_0_nonnull" >&6; } if test $ac_cv_func_malloc_0_nonnull = yes; then : gl_cv_func_malloc_0_nonnull=1 else gl_cv_func_malloc_0_nonnull=0 fi cat >>confdefs.h <<_ACEOF #define MALLOC_0_IS_NONNULL $gl_cv_func_malloc_0_nonnull _ACEOF { $as_echo "$as_me:${as_lineno-$LINENO}: checking for stdbool.h that conforms to C99" >&5 $as_echo_n "checking for stdbool.h that conforms to C99... " >&6; } if ${ac_cv_header_stdbool_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #ifdef __cplusplus typedef bool Bool; #else typedef _Bool Bool; #ifndef bool "error: bool is not defined" #endif #ifndef false "error: false is not defined" #endif #if false "error: false is not 0" #endif #ifndef true "error: true is not defined" #endif #if true != 1 "error: true is not 1" #endif #endif #ifndef __bool_true_false_are_defined "error: __bool_true_false_are_defined is not defined" #endif struct s { Bool s: 1; Bool t; bool u: 1; bool v; } s; char a[true == 1 ? 1 : -1]; char b[false == 0 ? 1 : -1]; char c[__bool_true_false_are_defined == 1 ? 1 : -1]; char d[(bool) 0.5 == true ? 1 : -1]; /* See body of main program for 'e'. */ char f[(Bool) 0.0 == false ? 1 : -1]; char g[true]; char h[sizeof (Bool)]; char i[sizeof s.t]; enum { j = false, k = true, l = false * true, m = true * 256 }; /* The following fails for HP aC++/ANSI C B3910B A.05.55 [Dec 04 2003]. */ Bool n[m]; char o[sizeof n == m * sizeof n[0] ? 1 : -1]; char p[-1 - (Bool) 0 < 0 && -1 - (bool) 0 < 0 ? 1 : -1]; /* Catch a bug in an HP-UX C compiler. See http://gcc.gnu.org/ml/gcc-patches/2003-12/msg02303.html http://lists.gnu.org/archive/html/bug-coreutils/2005-11/msg00161.html */ Bool q = true; Bool *pq = &q; bool *qq = &q; int main () { bool e = &s; *pq |= q; *pq |= ! q; *qq |= q; *qq |= ! q; /* Refer to every declared value, to avoid compiler optimizations. */ return (!a + !b + !c + !d + !e + !f + !g + !h + !i + !!j + !k + !!l + !m + !n + !o + !p + !q + !pq + !qq); ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_header_stdbool_h=yes else ac_cv_header_stdbool_h=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_header_stdbool_h" >&5 $as_echo "$ac_cv_header_stdbool_h" >&6; } ac_fn_c_check_type "$LINENO" "_Bool" "ac_cv_type__Bool" "$ac_includes_default" if test "x$ac_cv_type__Bool" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE__BOOL 1 _ACEOF fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for unsigned long long int" >&5 $as_echo_n "checking for unsigned long long int... " >&6; } if ${ac_cv_type_unsigned_long_long_int+:} false; then : $as_echo_n "(cached) " >&6 else ac_cv_type_unsigned_long_long_int=yes if test "x${ac_cv_prog_cc_c99-no}" = xno; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* For now, do not test the preprocessor; as of 2007 there are too many implementations with broken preprocessors. Perhaps this can be revisited in 2012. In the meantime, code should not expect #if to work with literals wider than 32 bits. */ /* Test literals. */ long long int ll = 9223372036854775807ll; long long int nll = -9223372036854775807LL; unsigned long long int ull = 18446744073709551615ULL; /* Test constant expressions. */ typedef int a[((-9223372036854775807LL < 0 && 0 < 9223372036854775807ll) ? 1 : -1)]; typedef int b[(18446744073709551615ULL <= (unsigned long long int) -1 ? 1 : -1)]; int i = 63; int main () { /* Test availability of runtime routines for shift and division. */ long long int llmax = 9223372036854775807ll; unsigned long long int ullmax = 18446744073709551615ull; return ((ll << 63) | (ll >> 63) | (ll < i) | (ll > i) | (llmax / ll) | (llmax % ll) | (ull << 63) | (ull >> 63) | (ull << i) | (ull >> i) | (ullmax / ull) | (ullmax % ull)); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : else ac_cv_type_unsigned_long_long_int=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_type_unsigned_long_long_int" >&5 $as_echo "$ac_cv_type_unsigned_long_long_int" >&6; } if test $ac_cv_type_unsigned_long_long_int = yes; then $as_echo "#define HAVE_UNSIGNED_LONG_LONG_INT 1" >>confdefs.h fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for long long int" >&5 $as_echo_n "checking for long long int... " >&6; } if ${ac_cv_type_long_long_int+:} false; then : $as_echo_n "(cached) " >&6 else ac_cv_type_long_long_int=yes if test "x${ac_cv_prog_cc_c99-no}" = xno; then ac_cv_type_long_long_int=$ac_cv_type_unsigned_long_long_int if test $ac_cv_type_long_long_int = yes; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #ifndef LLONG_MAX # define HALF \ (1LL << (sizeof (long long int) * CHAR_BIT - 2)) # define LLONG_MAX (HALF - 1 + HALF) #endif int main () { long long int n = 1; int i; for (i = 0; ; i++) { long long int m = n << i; if (m >> i != n) return 1; if (LLONG_MAX / 2 < m) break; } return 0; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : else ac_cv_type_long_long_int=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_type_long_long_int" >&5 $as_echo "$ac_cv_type_long_long_int" >&6; } if test $ac_cv_type_long_long_int = yes; then $as_echo "#define HAVE_LONG_LONG_INT 1" >>confdefs.h fi if test $ac_cv_type_long_long_int = yes; then HAVE_LONG_LONG_INT=1 else HAVE_LONG_LONG_INT=0 fi if test $ac_cv_type_unsigned_long_long_int = yes; then HAVE_UNSIGNED_LONG_LONG_INT=1 else HAVE_UNSIGNED_LONG_LONG_INT=0 fi if test $ac_cv_header_wchar_h = yes; then HAVE_WCHAR_H=1 else HAVE_WCHAR_H=0 fi if test $ac_cv_header_inttypes_h = yes; then HAVE_INTTYPES_H=1 else HAVE_INTTYPES_H=0 fi if test $ac_cv_header_sys_types_h = yes; then HAVE_SYS_TYPES_H=1 else HAVE_SYS_TYPES_H=0 fi if test $gl_cv_have_include_next = yes; then gl_cv_next_stdint_h='<'stdint.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_stdint_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_stdint_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'stdint.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_stdint_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_stdint_h gl_cv_next_stdint_h='"'$gl_header'"' else gl_cv_next_stdint_h='<'stdint.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_stdint_h" >&5 $as_echo "$gl_cv_next_stdint_h" >&6; } fi NEXT_STDINT_H=$gl_cv_next_stdint_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'stdint.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_stdint_h fi NEXT_AS_FIRST_DIRECTIVE_STDINT_H=$gl_next_as_first_directive if test $ac_cv_header_stdint_h = yes; then HAVE_STDINT_H=1 else HAVE_STDINT_H=0 fi if test $ac_cv_header_stdint_h = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether stdint.h conforms to C99" >&5 $as_echo_n "checking whether stdint.h conforms to C99... " >&6; } if ${gl_cv_header_working_stdint_h+:} false; then : $as_echo_n "(cached) " >&6 else gl_cv_header_working_stdint_h=no cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 /* work if build isn't clean */ #define __STDC_CONSTANT_MACROS 1 #define __STDC_LIMIT_MACROS 1 #include /* Dragonfly defines WCHAR_MIN, WCHAR_MAX only in . */ #if !(defined WCHAR_MIN && defined WCHAR_MAX) #error "WCHAR_MIN, WCHAR_MAX not defined in " #endif /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif #ifdef INT8_MAX int8_t a1 = INT8_MAX; int8_t a1min = INT8_MIN; #endif #ifdef INT16_MAX int16_t a2 = INT16_MAX; int16_t a2min = INT16_MIN; #endif #ifdef INT32_MAX int32_t a3 = INT32_MAX; int32_t a3min = INT32_MIN; #endif #ifdef INT64_MAX int64_t a4 = INT64_MAX; int64_t a4min = INT64_MIN; #endif #ifdef UINT8_MAX uint8_t b1 = UINT8_MAX; #else typedef int b1[(unsigned char) -1 != 255 ? 1 : -1]; #endif #ifdef UINT16_MAX uint16_t b2 = UINT16_MAX; #endif #ifdef UINT32_MAX uint32_t b3 = UINT32_MAX; #endif #ifdef UINT64_MAX uint64_t b4 = UINT64_MAX; #endif int_least8_t c1 = INT8_C (0x7f); int_least8_t c1max = INT_LEAST8_MAX; int_least8_t c1min = INT_LEAST8_MIN; int_least16_t c2 = INT16_C (0x7fff); int_least16_t c2max = INT_LEAST16_MAX; int_least16_t c2min = INT_LEAST16_MIN; int_least32_t c3 = INT32_C (0x7fffffff); int_least32_t c3max = INT_LEAST32_MAX; int_least32_t c3min = INT_LEAST32_MIN; int_least64_t c4 = INT64_C (0x7fffffffffffffff); int_least64_t c4max = INT_LEAST64_MAX; int_least64_t c4min = INT_LEAST64_MIN; uint_least8_t d1 = UINT8_C (0xff); uint_least8_t d1max = UINT_LEAST8_MAX; uint_least16_t d2 = UINT16_C (0xffff); uint_least16_t d2max = UINT_LEAST16_MAX; uint_least32_t d3 = UINT32_C (0xffffffff); uint_least32_t d3max = UINT_LEAST32_MAX; uint_least64_t d4 = UINT64_C (0xffffffffffffffff); uint_least64_t d4max = UINT_LEAST64_MAX; int_fast8_t e1 = INT_FAST8_MAX; int_fast8_t e1min = INT_FAST8_MIN; int_fast16_t e2 = INT_FAST16_MAX; int_fast16_t e2min = INT_FAST16_MIN; int_fast32_t e3 = INT_FAST32_MAX; int_fast32_t e3min = INT_FAST32_MIN; int_fast64_t e4 = INT_FAST64_MAX; int_fast64_t e4min = INT_FAST64_MIN; uint_fast8_t f1 = UINT_FAST8_MAX; uint_fast16_t f2 = UINT_FAST16_MAX; uint_fast32_t f3 = UINT_FAST32_MAX; uint_fast64_t f4 = UINT_FAST64_MAX; #ifdef INTPTR_MAX intptr_t g = INTPTR_MAX; intptr_t gmin = INTPTR_MIN; #endif #ifdef UINTPTR_MAX uintptr_t h = UINTPTR_MAX; #endif intmax_t i = INTMAX_MAX; uintmax_t j = UINTMAX_MAX; /* Check that SIZE_MAX has the correct type, if possible. */ #if 201112 <= __STDC_VERSION__ int k = _Generic (SIZE_MAX, size_t: 0); #elif (2 <= __GNUC__ || defined __IBM__TYPEOF__ \ || (0x5110 <= __SUNPRO_C && !__STDC__)) extern size_t k; extern __typeof__ (SIZE_MAX) k; #endif #include /* for CHAR_BIT */ #define TYPE_MINIMUM(t) \ ((t) ((t) 0 < (t) -1 ? (t) 0 : ~ TYPE_MAXIMUM (t))) #define TYPE_MAXIMUM(t) \ ((t) ((t) 0 < (t) -1 \ ? (t) -1 \ : ((((t) 1 << (sizeof (t) * CHAR_BIT - 2)) - 1) * 2 + 1))) struct s { int check_PTRDIFF: PTRDIFF_MIN == TYPE_MINIMUM (ptrdiff_t) && PTRDIFF_MAX == TYPE_MAXIMUM (ptrdiff_t) ? 1 : -1; /* Detect bug in FreeBSD 6.0 / ia64. */ int check_SIG_ATOMIC: SIG_ATOMIC_MIN == TYPE_MINIMUM (sig_atomic_t) && SIG_ATOMIC_MAX == TYPE_MAXIMUM (sig_atomic_t) ? 1 : -1; int check_SIZE: SIZE_MAX == TYPE_MAXIMUM (size_t) ? 1 : -1; int check_WCHAR: WCHAR_MIN == TYPE_MINIMUM (wchar_t) && WCHAR_MAX == TYPE_MAXIMUM (wchar_t) ? 1 : -1; /* Detect bug in mingw. */ int check_WINT: WINT_MIN == TYPE_MINIMUM (wint_t) && WINT_MAX == TYPE_MAXIMUM (wint_t) ? 1 : -1; /* Detect bugs in glibc 2.4 and Solaris 10 stdint.h, among others. */ int check_UINT8_C: (-1 < UINT8_C (0)) == (-1 < (uint_least8_t) 0) ? 1 : -1; int check_UINT16_C: (-1 < UINT16_C (0)) == (-1 < (uint_least16_t) 0) ? 1 : -1; /* Detect bugs in OpenBSD 3.9 stdint.h. */ #ifdef UINT8_MAX int check_uint8: (uint8_t) -1 == UINT8_MAX ? 1 : -1; #endif #ifdef UINT16_MAX int check_uint16: (uint16_t) -1 == UINT16_MAX ? 1 : -1; #endif #ifdef UINT32_MAX int check_uint32: (uint32_t) -1 == UINT32_MAX ? 1 : -1; #endif #ifdef UINT64_MAX int check_uint64: (uint64_t) -1 == UINT64_MAX ? 1 : -1; #endif int check_uint_least8: (uint_least8_t) -1 == UINT_LEAST8_MAX ? 1 : -1; int check_uint_least16: (uint_least16_t) -1 == UINT_LEAST16_MAX ? 1 : -1; int check_uint_least32: (uint_least32_t) -1 == UINT_LEAST32_MAX ? 1 : -1; int check_uint_least64: (uint_least64_t) -1 == UINT_LEAST64_MAX ? 1 : -1; int check_uint_fast8: (uint_fast8_t) -1 == UINT_FAST8_MAX ? 1 : -1; int check_uint_fast16: (uint_fast16_t) -1 == UINT_FAST16_MAX ? 1 : -1; int check_uint_fast32: (uint_fast32_t) -1 == UINT_FAST32_MAX ? 1 : -1; int check_uint_fast64: (uint_fast64_t) -1 == UINT_FAST64_MAX ? 1 : -1; int check_uintptr: (uintptr_t) -1 == UINTPTR_MAX ? 1 : -1; int check_uintmax: (uintmax_t) -1 == UINTMAX_MAX ? 1 : -1; int check_size: (size_t) -1 == SIZE_MAX ? 1 : -1; }; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : if test "$cross_compiling" = yes; then : gl_cv_header_working_stdint_h=yes else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 /* work if build isn't clean */ #define __STDC_CONSTANT_MACROS 1 #define __STDC_LIMIT_MACROS 1 #include /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif #include #include #define MVAL(macro) MVAL1(macro) #define MVAL1(expression) #expression static const char *macro_values[] = { #ifdef INT8_MAX MVAL (INT8_MAX), #endif #ifdef INT16_MAX MVAL (INT16_MAX), #endif #ifdef INT32_MAX MVAL (INT32_MAX), #endif #ifdef INT64_MAX MVAL (INT64_MAX), #endif #ifdef UINT8_MAX MVAL (UINT8_MAX), #endif #ifdef UINT16_MAX MVAL (UINT16_MAX), #endif #ifdef UINT32_MAX MVAL (UINT32_MAX), #endif #ifdef UINT64_MAX MVAL (UINT64_MAX), #endif NULL }; int main () { const char **mv; for (mv = macro_values; *mv != NULL; mv++) { const char *value = *mv; /* Test whether it looks like a cast expression. */ if (strncmp (value, "((unsigned int)"/*)*/, 15) == 0 || strncmp (value, "((unsigned short)"/*)*/, 17) == 0 || strncmp (value, "((unsigned char)"/*)*/, 16) == 0 || strncmp (value, "((int)"/*)*/, 6) == 0 || strncmp (value, "((signed short)"/*)*/, 15) == 0 || strncmp (value, "((signed char)"/*)*/, 14) == 0) return mv - macro_values + 1; } return 0; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_header_working_stdint_h=yes fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_working_stdint_h" >&5 $as_echo "$gl_cv_header_working_stdint_h" >&6; } fi HAVE_C99_STDINT_H=0 HAVE_SYS_BITYPES_H=0 HAVE_SYS_INTTYPES_H=0 STDINT_H=stdint.h if test "$gl_cv_header_working_stdint_h" = yes; then HAVE_C99_STDINT_H=1 { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether stdint.h predates C++11" >&5 $as_echo_n "checking whether stdint.h predates C++11... " >&6; } if ${gl_cv_header_stdint_predates_cxx11_h+:} false; then : $as_echo_n "(cached) " >&6 else gl_cv_header_stdint_predates_cxx11_h=yes cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 /* work if build isn't clean */ #include /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif intmax_t im = INTMAX_MAX; int32_t i32 = INT32_C (0x7fffffff); int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_stdint_predates_cxx11_h=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_stdint_predates_cxx11_h" >&5 $as_echo "$gl_cv_header_stdint_predates_cxx11_h" >&6; } if test "$gl_cv_header_stdint_predates_cxx11_h" = yes; then $as_echo "#define __STDC_CONSTANT_MACROS 1" >>confdefs.h $as_echo "#define __STDC_LIMIT_MACROS 1" >>confdefs.h fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether stdint.h has UINTMAX_WIDTH etc." >&5 $as_echo_n "checking whether stdint.h has UINTMAX_WIDTH etc.... " >&6; } if ${gl_cv_header_stdint_width+:} false; then : $as_echo_n "(cached) " >&6 else gl_cv_header_stdint_width=no cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Work if build is not clean. */ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 #ifndef __STDC_WANT_IEC_60559_BFP_EXT__ #define __STDC_WANT_IEC_60559_BFP_EXT__ 1 #endif #include /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif int iw = UINTMAX_WIDTH; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_stdint_width=yes fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_stdint_width" >&5 $as_echo "$gl_cv_header_stdint_width" >&6; } if test "$gl_cv_header_stdint_width" = yes; then STDINT_H= fi else for ac_header in sys/inttypes.h sys/bitypes.h do : as_ac_Header=`$as_echo "ac_cv_header_$ac_header" | $as_tr_sh` ac_fn_c_check_header_mongrel "$LINENO" "$ac_header" "$as_ac_Header" "$ac_includes_default" if eval test \"x\$"$as_ac_Header"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_$ac_header" | $as_tr_cpp` 1 _ACEOF fi done if test $ac_cv_header_sys_inttypes_h = yes; then HAVE_SYS_INTTYPES_H=1 fi if test $ac_cv_header_sys_bitypes_h = yes; then HAVE_SYS_BITYPES_H=1 fi if test $APPLE_UNIVERSAL_BUILD = 0; then for gltype in ptrdiff_t size_t ; do { $as_echo "$as_me:${as_lineno-$LINENO}: checking for bit size of $gltype" >&5 $as_echo_n "checking for bit size of $gltype... 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" >&6; } if eval \${gl_cv_type_${gltype}_suffix+:} false; then : $as_echo_n "(cached) " >&6 else eval gl_cv_type_${gltype}_suffix=no eval result=\$gl_cv_type_${gltype}_signed if test "$result" = yes; then glsufu= else glsufu=u fi for glsuf in "$glsufu" ${glsufu}l ${glsufu}ll ${glsufu}i64; do case $glsuf in '') gltype1='int';; l) gltype1='long int';; ll) gltype1='long long int';; i64) gltype1='__int64';; u) gltype1='unsigned int';; ul) gltype1='unsigned long int';; ull) gltype1='unsigned long long int';; ui64)gltype1='unsigned __int64';; esac cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif extern $gltype foo; extern $gltype1 foo; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval gl_cv_type_${gltype}_suffix=\$glsuf fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext eval result=\$gl_cv_type_${gltype}_suffix test "$result" != no && break done fi eval ac_res=\$gl_cv_type_${gltype}_suffix { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } GLTYPE=`echo $gltype | tr 'abcdefghijklmnopqrstuvwxyz ' 'ABCDEFGHIJKLMNOPQRSTUVWXYZ_'` eval result=\$gl_cv_type_${gltype}_suffix test "$result" = no && result= eval ${GLTYPE}_SUFFIX=\$result cat >>confdefs.h <<_ACEOF #define ${GLTYPE}_SUFFIX $result _ACEOF done fi for gltype in sig_atomic_t wchar_t wint_t ; do { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $gltype integer literal suffix" >&5 $as_echo_n "checking for $gltype integer literal suffix... 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LIMITS_H=limits.h if test -n "$LIMITS_H"; then GL_GENERATE_LIMITS_H_TRUE= GL_GENERATE_LIMITS_H_FALSE='#' else GL_GENERATE_LIMITS_H_TRUE='#' GL_GENERATE_LIMITS_H_FALSE= fi if test -n "$STDINT_H"; then GL_GENERATE_STDINT_H_TRUE= GL_GENERATE_STDINT_H_FALSE='#' else GL_GENERATE_STDINT_H_TRUE='#' GL_GENERATE_STDINT_H_FALSE= fi GNULIB_DPRINTF=0; GNULIB_FCLOSE=0; GNULIB_FDOPEN=0; GNULIB_FFLUSH=0; GNULIB_FGETC=0; GNULIB_FGETS=0; GNULIB_FOPEN=0; GNULIB_FPRINTF=0; GNULIB_FPRINTF_POSIX=0; GNULIB_FPURGE=0; GNULIB_FPUTC=0; GNULIB_FPUTS=0; GNULIB_FREAD=0; GNULIB_FREOPEN=0; GNULIB_FSCANF=0; GNULIB_FSEEK=0; GNULIB_FSEEKO=0; GNULIB_FTELL=0; GNULIB_FTELLO=0; GNULIB_FWRITE=0; GNULIB_GETC=0; GNULIB_GETCHAR=0; GNULIB_GETDELIM=0; GNULIB_GETLINE=0; GNULIB_OBSTACK_PRINTF=0; GNULIB_OBSTACK_PRINTF_POSIX=0; GNULIB_PCLOSE=0; GNULIB_PERROR=0; GNULIB_POPEN=0; GNULIB_PRINTF=0; GNULIB_PRINTF_POSIX=0; GNULIB_PUTC=0; GNULIB_PUTCHAR=0; GNULIB_PUTS=0; GNULIB_REMOVE=0; GNULIB_RENAME=0; GNULIB_RENAMEAT=0; GNULIB_SCANF=0; GNULIB_SNPRINTF=0; GNULIB_SPRINTF_POSIX=0; GNULIB_STDIO_H_NONBLOCKING=0; GNULIB_STDIO_H_SIGPIPE=0; GNULIB_TMPFILE=0; GNULIB_VASPRINTF=0; GNULIB_VFSCANF=0; GNULIB_VSCANF=0; GNULIB_VDPRINTF=0; GNULIB_VFPRINTF=0; GNULIB_VFPRINTF_POSIX=0; GNULIB_VPRINTF=0; GNULIB_VPRINTF_POSIX=0; GNULIB_VSNPRINTF=0; GNULIB_VSPRINTF_POSIX=0; HAVE_DECL_FPURGE=1; HAVE_DECL_FSEEKO=1; HAVE_DECL_FTELLO=1; HAVE_DECL_GETDELIM=1; HAVE_DECL_GETLINE=1; HAVE_DECL_OBSTACK_PRINTF=1; HAVE_DECL_SNPRINTF=1; HAVE_DECL_VSNPRINTF=1; HAVE_DPRINTF=1; HAVE_FSEEKO=1; HAVE_FTELLO=1; HAVE_PCLOSE=1; HAVE_POPEN=1; HAVE_RENAMEAT=1; HAVE_VASPRINTF=1; HAVE_VDPRINTF=1; REPLACE_DPRINTF=0; REPLACE_FCLOSE=0; REPLACE_FDOPEN=0; REPLACE_FFLUSH=0; REPLACE_FOPEN=0; REPLACE_FPRINTF=0; REPLACE_FPURGE=0; REPLACE_FREOPEN=0; REPLACE_FSEEK=0; REPLACE_FSEEKO=0; REPLACE_FTELL=0; REPLACE_FTELLO=0; REPLACE_GETDELIM=0; REPLACE_GETLINE=0; REPLACE_OBSTACK_PRINTF=0; REPLACE_PERROR=0; REPLACE_POPEN=0; REPLACE_PRINTF=0; REPLACE_REMOVE=0; REPLACE_RENAME=0; REPLACE_RENAMEAT=0; REPLACE_SNPRINTF=0; REPLACE_SPRINTF=0; REPLACE_STDIO_READ_FUNCS=0; REPLACE_STDIO_WRITE_FUNCS=0; REPLACE_TMPFILE=0; REPLACE_VASPRINTF=0; REPLACE_VDPRINTF=0; REPLACE_VFPRINTF=0; REPLACE_VPRINTF=0; REPLACE_VSNPRINTF=0; REPLACE_VSPRINTF=0; GNULIB_FFS=0; HAVE_FFS=1; HAVE_STRCASECMP=1; HAVE_DECL_STRNCASECMP=1; REPLACE_STRERROR_0=0 { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether strerror(0) succeeds" >&5 $as_echo_n "checking whether strerror(0) succeeds... " >&6; } if ${gl_cv_func_strerror_0_works+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_strerror_0_works="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_strerror_0_works="guessing no" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int main () { int result = 0; char *str; errno = 0; str = strerror (0); if (!*str) result |= 1; if (errno) result |= 2; if (strstr (str, "nknown") || strstr (str, "ndefined")) result |= 4; return result; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_strerror_0_works=yes else gl_cv_func_strerror_0_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_strerror_0_works" >&5 $as_echo "$gl_cv_func_strerror_0_works" >&6; } case "$gl_cv_func_strerror_0_works" in *yes) ;; *) REPLACE_STRERROR_0=1 $as_echo "#define REPLACE_STRERROR_0 1" >>confdefs.h ;; esac if test $gl_cv_have_include_next = yes; then gl_cv_next_string_h='<'string.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_string_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'string.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_string_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_string_h gl_cv_next_string_h='"'$gl_header'"' fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_string_h" >&5 $as_echo "$gl_cv_next_string_h" >&6; } fi NEXT_STRING_H=$gl_cv_next_string_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'string.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_string_h fi NEXT_AS_FIRST_DIRECTIVE_STRING_H=$gl_next_as_first_directive for gl_func in ffsl ffsll memmem mempcpy memrchr rawmemchr stpcpy stpncpy strchrnul strdup strncat strndup strnlen strpbrk strsep strcasestr strtok_r strerror_r strsignal strverscmp; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done if test $gl_cv_have_include_next = yes; then gl_cv_next_strings_h='<'strings.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_strings_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_strings_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'strings.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_strings_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_strings_h gl_cv_next_strings_h='"'$gl_header'"' else gl_cv_next_strings_h='<'strings.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_strings_h" >&5 $as_echo "$gl_cv_next_strings_h" >&6; } fi NEXT_STRINGS_H=$gl_cv_next_strings_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'strings.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_strings_h fi NEXT_AS_FIRST_DIRECTIVE_STRINGS_H=$gl_next_as_first_directive if test $ac_cv_header_strings_h = yes; then HAVE_STRINGS_H=1 else HAVE_STRINGS_H=0 fi for gl_func in ffs strcasecmp strncasecmp; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Minix 3.1.8 has a bug: must be included before . */ #include #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done ac_fn_c_check_decl "$LINENO" "strndup" "ac_cv_have_decl_strndup" "$ac_includes_default" if test "x$ac_cv_have_decl_strndup" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_STRNDUP $ac_have_decl _ACEOF ac_fn_c_check_decl "$LINENO" "strnlen" "ac_cv_have_decl_strnlen" "$ac_includes_default" if test "x$ac_cv_have_decl_strnlen" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_STRNLEN $ac_have_decl _ACEOF ac_fn_c_check_type "$LINENO" "pid_t" "ac_cv_type_pid_t" "$ac_includes_default" if test "x$ac_cv_type_pid_t" = xyes; then : else cat >>confdefs.h <<_ACEOF #define pid_t int _ACEOF fi ac_fn_c_check_type "$LINENO" "mode_t" "ac_cv_type_mode_t" "$ac_includes_default" if test "x$ac_cv_type_mode_t" = xyes; then : else cat >>confdefs.h <<_ACEOF #define mode_t int _ACEOF fi case "$host_os" in mingw*) { $as_echo "$as_me:${as_lineno-$LINENO}: checking for 64-bit off_t" >&5 $as_echo_n "checking for 64-bit off_t... " >&6; } if ${gl_cv_type_off_t_64+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int verify_off_t_size[sizeof (off_t) >= 8 ? 1 : -1]; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_type_off_t_64=yes else gl_cv_type_off_t_64=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_type_off_t_64" >&5 $as_echo "$gl_cv_type_off_t_64" >&6; } if test $gl_cv_type_off_t_64 = no; then WINDOWS_64_BIT_OFF_T=1 else WINDOWS_64_BIT_OFF_T=0 fi WINDOWS_64_BIT_ST_SIZE=1 ;; *) WINDOWS_64_BIT_OFF_T=0 WINDOWS_64_BIT_ST_SIZE=0 ;; esac if test $gl_cv_have_include_next = yes; then gl_cv_next_sys_types_h='<'sys/types.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_sys_types_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'sys/types.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_sys_types_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_sys_types_h gl_cv_next_sys_types_h='"'$gl_header'"' fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_sys_types_h" >&5 $as_echo "$gl_cv_next_sys_types_h" >&6; } fi NEXT_SYS_TYPES_H=$gl_cv_next_sys_types_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'sys/types.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_sys_types_h fi NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H=$gl_next_as_first_directive { $as_echo "$as_me:${as_lineno-$LINENO}: checking for wint_t" >&5 $as_echo_n "checking for wint_t... " >&6; } if ${gt_cv_c_wint_t+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include wint_t foo = (wchar_t)'\0'; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gt_cv_c_wint_t=yes else gt_cv_c_wint_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_c_wint_t" >&5 $as_echo "$gt_cv_c_wint_t" >&6; } if test $gt_cv_c_wint_t = yes; then $as_echo "#define HAVE_WINT_T 1" >>confdefs.h fi if test $ac_cv_header_features_h = yes; then HAVE_FEATURES_H=1 else HAVE_FEATURES_H=0 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for inttypes.h" >&5 $as_echo_n "checking for inttypes.h... " >&6; } if ${gl_cv_header_inttypes_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int main () { uintmax_t i = (uintmax_t) -1; return !i; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_inttypes_h=yes else gl_cv_header_inttypes_h=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_inttypes_h" >&5 $as_echo "$gl_cv_header_inttypes_h" >&6; } if test $gl_cv_header_inttypes_h = yes; then cat >>confdefs.h <<_ACEOF #define HAVE_INTTYPES_H_WITH_UINTMAX 1 _ACEOF fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for stdint.h" >&5 $as_echo_n "checking for stdint.h... " >&6; } if ${gl_cv_header_stdint_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int main () { uintmax_t i = (uintmax_t) -1; return !i; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_stdint_h=yes else gl_cv_header_stdint_h=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_stdint_h" >&5 $as_echo "$gl_cv_header_stdint_h" >&6; } if test $gl_cv_header_stdint_h = yes; then cat >>confdefs.h <<_ACEOF #define HAVE_STDINT_H_WITH_UINTMAX 1 _ACEOF fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for intmax_t" >&5 $as_echo_n "checking for intmax_t... " >&6; } if ${gt_cv_c_intmax_t+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_STDINT_H_WITH_UINTMAX #include #endif #if HAVE_INTTYPES_H_WITH_UINTMAX #include #endif int main () { intmax_t x = -1; return !x; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gt_cv_c_intmax_t=yes else gt_cv_c_intmax_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_c_intmax_t" >&5 $as_echo "$gt_cv_c_intmax_t" >&6; } if test $gt_cv_c_intmax_t = yes; then $as_echo "#define HAVE_INTMAX_T 1" >>confdefs.h else test $ac_cv_type_long_long_int = yes \ && ac_type='long long' \ || ac_type='long' cat >>confdefs.h <<_ACEOF #define intmax_t $ac_type _ACEOF fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking where to find the exponent in a 'double'" >&5 $as_echo_n "checking where to find the exponent in a 'double'... " >&6; } if ${gl_cv_cc_double_expbit0+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if defined arm || defined __arm || defined __arm__ mixed_endianness #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "mixed_endianness" >/dev/null 2>&1; then : gl_cv_cc_double_expbit0="unknown" else : if ${ac_cv_c_bigendian+:} false; then : $as_echo_n "(cached) " >&6 else ac_cv_c_bigendian=unknown # See if we're dealing with a universal compiler. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifndef __APPLE_CC__ not a universal capable compiler #endif typedef int dummy; _ACEOF if ac_fn_c_try_compile "$LINENO"; then : # Check for potential -arch flags. It is not universal unless # there are at least two -arch flags with different values. ac_arch= ac_prev= for ac_word in $CC $CFLAGS $CPPFLAGS $LDFLAGS; do if test -n "$ac_prev"; then case $ac_word in i?86 | x86_64 | ppc | ppc64) if test -z "$ac_arch" || test "$ac_arch" = "$ac_word"; then ac_arch=$ac_word else ac_cv_c_bigendian=universal break fi ;; esac ac_prev= elif test "x$ac_word" = "x-arch"; then ac_prev=arch fi done fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext if test $ac_cv_c_bigendian = unknown; then # See if sys/param.h defines the BYTE_ORDER macro. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int main () { #if ! (defined BYTE_ORDER && defined BIG_ENDIAN \ && defined LITTLE_ENDIAN && BYTE_ORDER && BIG_ENDIAN \ && LITTLE_ENDIAN) bogus endian macros #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : # It does; now see whether it defined to BIG_ENDIAN or not. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int main () { #if BYTE_ORDER != BIG_ENDIAN not big endian #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_c_bigendian=yes else ac_cv_c_bigendian=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi if test $ac_cv_c_bigendian = unknown; then # See if defines _LITTLE_ENDIAN or _BIG_ENDIAN (e.g., Solaris). cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #if ! (defined _LITTLE_ENDIAN || defined _BIG_ENDIAN) bogus endian macros #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : # It does; now see whether it defined to _BIG_ENDIAN or not. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #ifndef _BIG_ENDIAN not big endian #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_c_bigendian=yes else ac_cv_c_bigendian=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi if test $ac_cv_c_bigendian = unknown; then # Compile a test program. if test "$cross_compiling" = yes; then : # Try to guess by grepping values from an object file. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ short int ascii_mm[] = { 0x4249, 0x4765, 0x6E44, 0x6961, 0x6E53, 0x7953, 0 }; short int ascii_ii[] = { 0x694C, 0x5454, 0x656C, 0x6E45, 0x6944, 0x6E61, 0 }; int use_ascii (int i) { return ascii_mm[i] + ascii_ii[i]; } short int ebcdic_ii[] = { 0x89D3, 0xE3E3, 0x8593, 0x95C5, 0x89C4, 0x9581, 0 }; short int ebcdic_mm[] = { 0xC2C9, 0xC785, 0x95C4, 0x8981, 0x95E2, 0xA8E2, 0 }; int use_ebcdic (int i) { return ebcdic_mm[i] + ebcdic_ii[i]; } extern int foo; int main () { return use_ascii (foo) == use_ebcdic (foo); ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : if grep BIGenDianSyS conftest.$ac_objext >/dev/null; then ac_cv_c_bigendian=yes fi if grep LiTTleEnDian conftest.$ac_objext >/dev/null ; then if test "$ac_cv_c_bigendian" = unknown; then ac_cv_c_bigendian=no else # finding both strings is unlikely to happen, but who knows? ac_cv_c_bigendian=unknown fi fi fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ $ac_includes_default int main () { /* Are we little or big endian? From Harbison&Steele. */ union { long int l; char c[sizeof (long int)]; } u; u.l = 1; return u.c[sizeof (long int) - 1] == 1; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : ac_cv_c_bigendian=no else ac_cv_c_bigendian=yes fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi : case $ac_cv_c_bigendian in #( yes) gl_cv_cc_double_expbit0="word 0 bit 20";; #( no) gl_cv_cc_double_expbit0="word 1 bit 20" ;; #( universal) $as_echo "#define AC_APPLE_UNIVERSAL_BUILD 1" >>confdefs.h ;; #( *) gl_cv_cc_double_expbit0="unknown" ;; esac fi rm -f conftest* else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #include #define NWORDS \ ((sizeof (double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { double value; unsigned int word[NWORDS]; } memory_double; static unsigned int ored_words[NWORDS]; static unsigned int anded_words[NWORDS]; static void add_to_ored_words (double x) { memory_double m; size_t i; /* Clear it first, in case sizeof (double) < sizeof (memory_double). */ memset (&m, 0, sizeof (memory_double)); m.value = x; for (i = 0; i < NWORDS; i++) { ored_words[i] |= m.word[i]; anded_words[i] &= m.word[i]; } } int main () { size_t j; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; for (j = 0; j < NWORDS; j++) anded_words[j] = ~ (unsigned int) 0; add_to_ored_words (0.25); add_to_ored_words (0.5); add_to_ored_words (1.0); add_to_ored_words (2.0); add_to_ored_words (4.0); /* Remove bits that are common (e.g. if representation of the first mantissa bit is explicit). */ for (j = 0; j < NWORDS; j++) ored_words[j] &= ~anded_words[j]; /* Now find the nonzero word. */ for (j = 0; j < NWORDS; j++) if (ored_words[j] != 0) break; if (j < NWORDS) { size_t i; for (i = j + 1; i < NWORDS; i++) if (ored_words[i] != 0) { fprintf (fp, "unknown"); return (fclose (fp) != 0); } for (i = 0; ; i++) if ((ored_words[j] >> i) & 1) { fprintf (fp, "word %d bit %d", (int) j, (int) i); return (fclose (fp) != 0); } } fprintf (fp, "unknown"); return (fclose (fp) != 0); } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_cc_double_expbit0=`cat conftest.out` else gl_cv_cc_double_expbit0="unknown" fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.out fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_cc_double_expbit0" >&5 $as_echo "$gl_cv_cc_double_expbit0" >&6; } case "$gl_cv_cc_double_expbit0" in word*bit*) word=`echo "$gl_cv_cc_double_expbit0" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$gl_cv_cc_double_expbit0" | sed -e 's/word.*bit //'` cat >>confdefs.h <<_ACEOF #define DBL_EXPBIT0_WORD $word _ACEOF cat >>confdefs.h <<_ACEOF #define DBL_EXPBIT0_BIT $bit _ACEOF ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether snprintf returns a byte count as in C99" >&5 $as_echo_n "checking whether snprintf returns a byte count as in C99... " >&6; } if ${gl_cv_func_snprintf_retval_c99+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on FreeBSD >= 5. freebsd[1-4].*) gl_cv_func_snprintf_retval_c99="guessing no";; freebsd* | kfreebsd*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_snprintf_retval_c99="guessing no";; darwin*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on OpenBSD >= 3.9. openbsd[1-2].* | openbsd3.[0-8] | openbsd3.[0-8].*) gl_cv_func_snprintf_retval_c99="guessing no";; openbsd*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on Solaris >= 2.10. solaris2.[1-9][0-9]*) gl_cv_func_printf_sizes_c99="guessing yes";; solaris*) gl_cv_func_printf_sizes_c99="guessing no";; # Guess yes on AIX >= 4. aix[1-3]*) gl_cv_func_snprintf_retval_c99="guessing no";; aix*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on NetBSD >= 3. netbsd[1-2]* | netbsdelf[1-2]* | netbsdaout[1-2]* | netbsdcoff[1-2]*) gl_cv_func_snprintf_retval_c99="guessing no";; netbsd*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_snprintf_retval_c99="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_snprintf_retval_c99="guessing no";; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_SNPRINTF # define my_snprintf snprintf #else # include static int my_snprintf (char *buf, int size, const char *format, ...) { va_list args; int ret; va_start (args, format); ret = vsnprintf (buf, size, format, args); va_end (args); return ret; } #endif static char buf[100]; int main () { strcpy (buf, "ABCDEF"); if (my_snprintf (buf, 3, "%d %d", 4567, 89) != 7) return 1; if (my_snprintf (buf, 0, "%d %d", 4567, 89) != 7) return 2; if (my_snprintf (NULL, 0, "%d %d", 4567, 89) != 7) return 3; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_snprintf_retval_c99=yes else gl_cv_func_snprintf_retval_c99=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_snprintf_retval_c99" >&5 $as_echo "$gl_cv_func_snprintf_retval_c99" >&6; } for ac_func in snprintf strnlen wcslen wcsnlen mbrtowc wcrtomb do : as_ac_var=`$as_echo "ac_cv_func_$ac_func" | $as_tr_sh` ac_fn_c_check_func "$LINENO" "$ac_func" "$as_ac_var" if eval test \"x\$"$as_ac_var"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_$ac_func" | $as_tr_cpp` 1 _ACEOF fi done ac_fn_c_check_decl "$LINENO" "_snprintf" "ac_cv_have_decl__snprintf" "#include " if test "x$ac_cv_have_decl__snprintf" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL__SNPRINTF $ac_have_decl _ACEOF case "$gl_cv_func_snprintf_retval_c99" in *yes) $as_echo "#define HAVE_SNPRINTF_RETVAL_C99 1" >>confdefs.h ;; esac ac_fn_c_check_decl "$LINENO" "vsnprintf" "ac_cv_have_decl_vsnprintf" "$ac_includes_default" if test "x$ac_cv_have_decl_vsnprintf" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_VSNPRINTF $ac_have_decl _ACEOF GNULIB_ISWBLANK=0; GNULIB_WCTYPE=0; GNULIB_ISWCTYPE=0; GNULIB_WCTRANS=0; GNULIB_TOWCTRANS=0; HAVE_ISWBLANK=1; HAVE_WCTYPE_T=1; HAVE_WCTRANS_T=1; REPLACE_ISWBLANK=0; GNULIB_ISBLANK=0; HAVE_ISBLANK=1; { $as_echo "$as_me:${as_lineno-$LINENO}: checking if environ is properly declared" >&5 $as_echo_n "checking if environ is properly declared... " >&6; } if ${gt_cv_var_environ_declaration+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if HAVE_UNISTD_H #include #endif /* mingw, BeOS, Haiku declare environ in , not in . */ #include extern struct { int foo; } environ; int main () { environ.foo = 1; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gt_cv_var_environ_declaration=no else gt_cv_var_environ_declaration=yes fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_var_environ_declaration" >&5 $as_echo "$gt_cv_var_environ_declaration" >&6; } if test $gt_cv_var_environ_declaration = yes; then $as_echo "#define HAVE_ENVIRON_DECL 1" >>confdefs.h fi if test $gt_cv_var_environ_declaration != yes; then HAVE_DECL_ENVIRON=0 fi GNULIB_FCNTL=0; GNULIB_NONBLOCKING=0; GNULIB_OPEN=0; GNULIB_OPENAT=0; HAVE_FCNTL=1; HAVE_OPENAT=1; REPLACE_FCNTL=0; REPLACE_OPEN=0; REPLACE_OPENAT=0; GNULIB_FCHMODAT=0; GNULIB_FSTAT=0; GNULIB_FSTATAT=0; GNULIB_FUTIMENS=0; GNULIB_LCHMOD=0; GNULIB_LSTAT=0; GNULIB_MKDIRAT=0; GNULIB_MKFIFO=0; GNULIB_MKFIFOAT=0; GNULIB_MKNOD=0; GNULIB_MKNODAT=0; GNULIB_STAT=0; GNULIB_UTIMENSAT=0; HAVE_FCHMODAT=1; HAVE_FSTATAT=1; HAVE_FUTIMENS=1; HAVE_LCHMOD=1; HAVE_LSTAT=1; HAVE_MKDIRAT=1; HAVE_MKFIFO=1; HAVE_MKFIFOAT=1; HAVE_MKNOD=1; HAVE_MKNODAT=1; HAVE_UTIMENSAT=1; REPLACE_FSTAT=0; REPLACE_FSTATAT=0; REPLACE_FUTIMENS=0; REPLACE_LSTAT=0; REPLACE_MKDIR=0; REPLACE_MKFIFO=0; REPLACE_MKNOD=0; REPLACE_STAT=0; REPLACE_UTIMENSAT=0; { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether stat file-mode macros are broken" >&5 $as_echo_n "checking whether stat file-mode macros are broken... " >&6; } if ${ac_cv_header_stat_broken+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if defined S_ISBLK && defined S_IFDIR extern char c1[S_ISBLK (S_IFDIR) ? -1 : 1]; #endif #if defined S_ISBLK && defined S_IFCHR extern char c2[S_ISBLK (S_IFCHR) ? -1 : 1]; #endif #if defined S_ISLNK && defined S_IFREG extern char c3[S_ISLNK (S_IFREG) ? -1 : 1]; #endif #if defined S_ISSOCK && defined S_IFREG extern char c4[S_ISSOCK (S_IFREG) ? -1 : 1]; #endif _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_header_stat_broken=no else ac_cv_header_stat_broken=yes fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_header_stat_broken" >&5 $as_echo "$ac_cv_header_stat_broken" >&6; } if test $ac_cv_header_stat_broken = yes; then $as_echo "#define STAT_MACROS_BROKEN 1" >>confdefs.h fi if test $gl_cv_have_include_next = yes; then gl_cv_next_sys_stat_h='<'sys/stat.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_sys_stat_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_sys_stat_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'sys/stat.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_sys_stat_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_sys_stat_h gl_cv_next_sys_stat_h='"'$gl_header'"' else gl_cv_next_sys_stat_h='<'sys/stat.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_sys_stat_h" >&5 $as_echo "$gl_cv_next_sys_stat_h" >&6; } fi NEXT_SYS_STAT_H=$gl_cv_next_sys_stat_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'sys/stat.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_sys_stat_h fi NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H=$gl_next_as_first_directive if test $WINDOWS_64_BIT_ST_SIZE = 1; then $as_echo "#define _GL_WINDOWS_64_BIT_ST_SIZE 1" >>confdefs.h fi ac_fn_c_check_type "$LINENO" "nlink_t" "ac_cv_type_nlink_t" "#include #include " if test "x$ac_cv_type_nlink_t" = xyes; then : else $as_echo "#define nlink_t int" >>confdefs.h fi for gl_func in fchmodat fstat fstatat futimens lchmod lstat mkdirat mkfifo mkfifoat mknod mknodat stat utimensat; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... 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" >&6; } if ${gl_cv_func_getcwd_null+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_getcwd_null="guessing yes";; # Guess yes on Cygwin. cygwin*) gl_cv_func_getcwd_null="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_getcwd_null="guessing no";; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ # include # if HAVE_UNISTD_H # include # else /* on Windows with MSVC */ # include # endif # ifndef getcwd char *getcwd (); # endif int main () { #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* mingw cwd does not start with '/', but getcwd does allocate. However, mingw fails to honor non-zero size. */ #else if (chdir ("/") != 0) return 1; else { char *f = getcwd (NULL, 0); if (! f) return 2; if (f[0] != '/') return 3; if (f[1] != '\0') return 4; free (f); return 0; } #endif ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_getcwd_null=yes else gl_cv_func_getcwd_null=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_getcwd_null" >&5 $as_echo "$gl_cv_func_getcwd_null" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking for getcwd with POSIX signature" >&5 $as_echo_n "checking for getcwd with POSIX signature... " >&6; } if ${gl_cv_func_getcwd_posix_signature+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { extern #ifdef __cplusplus "C" #endif char *getcwd (char *, size_t); ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_func_getcwd_posix_signature=yes else gl_cv_func_getcwd_posix_signature=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_getcwd_posix_signature" >&5 $as_echo "$gl_cv_func_getcwd_posix_signature" >&6; } ac_fn_c_check_decl "$LINENO" "getdtablesize" "ac_cv_have_decl_getdtablesize" "$ac_includes_default" if test "x$ac_cv_have_decl_getdtablesize" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_GETDTABLESIZE $ac_have_decl _ACEOF GNULIB_GETTIMEOFDAY=0; HAVE_GETTIMEOFDAY=1; HAVE_STRUCT_TIMEVAL=1; HAVE_SYS_TIME_H=1; HAVE_TIMEZONE_T=0; REPLACE_GETTIMEOFDAY=0; REPLACE_STRUCT_TIMEVAL=0; if test $gl_cv_have_include_next = yes; then gl_cv_next_sys_time_h='<'sys/time.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_sys_time_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_sys_time_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'sys/time.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_sys_time_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_sys_time_h gl_cv_next_sys_time_h='"'$gl_header'"' else gl_cv_next_sys_time_h='<'sys/time.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_sys_time_h" >&5 $as_echo "$gl_cv_next_sys_time_h" >&6; } fi NEXT_SYS_TIME_H=$gl_cv_next_sys_time_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'sys/time.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_sys_time_h fi NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H=$gl_next_as_first_directive if test $ac_cv_header_sys_time_h != yes; then HAVE_SYS_TIME_H=0 fi if test $ac_cv_header_sys_socket_h != yes; then for ac_header in winsock2.h do : ac_fn_c_check_header_mongrel "$LINENO" "winsock2.h" "ac_cv_header_winsock2_h" "$ac_includes_default" if test "x$ac_cv_header_winsock2_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_WINSOCK2_H 1 _ACEOF fi done fi if test "$ac_cv_header_winsock2_h" = yes; then HAVE_WINSOCK2_H=1 UNISTD_H_HAVE_WINSOCK2_H=1 SYS_IOCTL_H_HAVE_WINSOCK2_H=1 else HAVE_WINSOCK2_H=0 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for struct timeval" >&5 $as_echo_n "checking for struct timeval... " >&6; } if ${gl_cv_sys_struct_timeval+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if HAVE_SYS_TIME_H #include #endif #include #if HAVE_WINSOCK2_H # include #endif int main () { static struct timeval x; x.tv_sec = x.tv_usec; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_sys_struct_timeval=yes else gl_cv_sys_struct_timeval=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_sys_struct_timeval" >&5 $as_echo "$gl_cv_sys_struct_timeval" >&6; } if test $gl_cv_sys_struct_timeval != yes; then HAVE_STRUCT_TIMEVAL=0 else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for wide-enough struct timeval.tv_sec member" >&5 $as_echo_n "checking for wide-enough struct timeval.tv_sec member... " >&6; } if ${gl_cv_sys_struct_timeval_tv_sec+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if HAVE_SYS_TIME_H #include #endif #include #if HAVE_WINSOCK2_H # include #endif int main () { static struct timeval x; typedef int verify_tv_sec_type[ sizeof (time_t) <= sizeof x.tv_sec ? 1 : -1 ]; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_sys_struct_timeval_tv_sec=yes else gl_cv_sys_struct_timeval_tv_sec=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_sys_struct_timeval_tv_sec" >&5 $as_echo "$gl_cv_sys_struct_timeval_tv_sec" >&6; } if test $gl_cv_sys_struct_timeval_tv_sec != yes; then REPLACE_STRUCT_TIMEVAL=1 fi fi for gl_func in gettimeofday; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if HAVE_SYS_TIME_H # include #endif #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done GNULIB_IMAXABS=0; GNULIB_IMAXDIV=0; GNULIB_STRTOIMAX=0; GNULIB_STRTOUMAX=0; HAVE_DECL_IMAXABS=1; HAVE_DECL_IMAXDIV=1; HAVE_DECL_STRTOIMAX=1; HAVE_DECL_STRTOUMAX=1; REPLACE_STRTOIMAX=0; REPLACE_STRTOUMAX=0; INT32_MAX_LT_INTMAX_MAX=1; INT64_MAX_EQ_LONG_MAX='defined _LP64'; PRI_MACROS_BROKEN=0; PRIPTR_PREFIX=__PRIPTR_PREFIX; UINT32_MAX_LT_UINTMAX_MAX=1; UINT64_MAX_EQ_ULONG_MAX='defined _LP64'; if test $gl_cv_have_include_next = yes; then gl_cv_next_inttypes_h='<'inttypes.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_inttypes_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_inttypes_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'inttypes.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_inttypes_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_inttypes_h gl_cv_next_inttypes_h='"'$gl_header'"' else gl_cv_next_inttypes_h='<'inttypes.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_inttypes_h" >&5 $as_echo "$gl_cv_next_inttypes_h" >&6; } fi NEXT_INTTYPES_H=$gl_cv_next_inttypes_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'inttypes.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_inttypes_h fi NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H=$gl_next_as_first_directive for gl_func in imaxabs imaxdiv strtoimax strtoumax; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done for ac_header in inttypes.h do : ac_fn_c_check_header_mongrel "$LINENO" "inttypes.h" "ac_cv_header_inttypes_h" "$ac_includes_default" if test "x$ac_cv_header_inttypes_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_INTTYPES_H 1 _ACEOF fi done if test $ac_cv_header_inttypes_h = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether the inttypes.h PRIxNN macros are broken" >&5 $as_echo_n "checking whether the inttypes.h PRIxNN macros are broken... " >&6; } if ${gt_cv_inttypes_pri_broken+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #ifdef PRId32 char *p = PRId32; #endif int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gt_cv_inttypes_pri_broken=no else gt_cv_inttypes_pri_broken=yes fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_inttypes_pri_broken" >&5 $as_echo "$gt_cv_inttypes_pri_broken" >&6; } fi if test "$gt_cv_inttypes_pri_broken" = yes; then cat >>confdefs.h <<_ACEOF #define PRI_MACROS_BROKEN 1 _ACEOF PRI_MACROS_BROKEN=1 else PRI_MACROS_BROKEN=0 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for LC_MESSAGES" >&5 $as_echo_n "checking for LC_MESSAGES... " >&6; } if ${gt_cv_val_LC_MESSAGES+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { return LC_MESSAGES ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gt_cv_val_LC_MESSAGES=yes else gt_cv_val_LC_MESSAGES=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_val_LC_MESSAGES" >&5 $as_echo "$gt_cv_val_LC_MESSAGES" >&6; } if test $gt_cv_val_LC_MESSAGES = yes; then $as_echo "#define HAVE_LC_MESSAGES 1" >>confdefs.h fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for CFPreferencesCopyAppValue" >&5 $as_echo_n "checking for CFPreferencesCopyAppValue... " >&6; } if ${gt_cv_func_CFPreferencesCopyAppValue+:} false; then : $as_echo_n "(cached) " >&6 else gt_save_LIBS="$LIBS" LIBS="$LIBS -Wl,-framework -Wl,CoreFoundation" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { CFPreferencesCopyAppValue(NULL, NULL) ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gt_cv_func_CFPreferencesCopyAppValue=yes else gt_cv_func_CFPreferencesCopyAppValue=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS="$gt_save_LIBS" fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_func_CFPreferencesCopyAppValue" >&5 $as_echo "$gt_cv_func_CFPreferencesCopyAppValue" >&6; } if test $gt_cv_func_CFPreferencesCopyAppValue = yes; then $as_echo "#define HAVE_CFPREFERENCESCOPYAPPVALUE 1" >>confdefs.h fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for CFLocaleCopyCurrent" >&5 $as_echo_n "checking for CFLocaleCopyCurrent... " >&6; } if ${gt_cv_func_CFLocaleCopyCurrent+:} false; then : $as_echo_n "(cached) " >&6 else gt_save_LIBS="$LIBS" LIBS="$LIBS -Wl,-framework -Wl,CoreFoundation" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { CFLocaleCopyCurrent(); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gt_cv_func_CFLocaleCopyCurrent=yes else gt_cv_func_CFLocaleCopyCurrent=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS="$gt_save_LIBS" fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_func_CFLocaleCopyCurrent" >&5 $as_echo "$gt_cv_func_CFLocaleCopyCurrent" >&6; } if test $gt_cv_func_CFLocaleCopyCurrent = yes; then $as_echo "#define HAVE_CFLOCALECOPYCURRENT 1" >>confdefs.h fi INTL_MACOSX_LIBS= if test $gt_cv_func_CFPreferencesCopyAppValue = yes || test $gt_cv_func_CFLocaleCopyCurrent = yes; then INTL_MACOSX_LIBS="-Wl,-framework -Wl,CoreFoundation" fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether lstat correctly handles trailing slash" >&5 $as_echo_n "checking whether lstat correctly handles trailing slash... " >&6; } if ${gl_cv_func_lstat_dereferences_slashed_symlink+:} false; then : $as_echo_n "(cached) " >&6 else rm -f conftest.sym conftest.file echo >conftest.file if test "$cross_compiling" = yes; then : case "$host_os" in *-gnu*) # Guess yes on glibc systems. gl_cv_func_lstat_dereferences_slashed_symlink="guessing yes" ;; *) # If we don't know, assume the worst. gl_cv_func_lstat_dereferences_slashed_symlink="guessing no" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ $ac_includes_default int main () { struct stat sbuf; if (symlink ("conftest.file", "conftest.sym") != 0) return 1; /* Linux will dereference the symlink and fail, as required by POSIX. That is better in the sense that it means we will not have to compile and use the lstat wrapper. */ return lstat ("conftest.sym/", &sbuf) == 0; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_lstat_dereferences_slashed_symlink=yes else gl_cv_func_lstat_dereferences_slashed_symlink=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.sym conftest.file fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_lstat_dereferences_slashed_symlink" >&5 $as_echo "$gl_cv_func_lstat_dereferences_slashed_symlink" >&6; } case "$gl_cv_func_lstat_dereferences_slashed_symlink" in *yes) cat >>confdefs.h <<_ACEOF #define LSTAT_FOLLOWS_SLASHED_SYMLINK 1 _ACEOF ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking for promoted mode_t type" >&5 $as_echo_n "checking for promoted mode_t type... " >&6; } if ${gl_cv_promoted_mode_t+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { typedef int array[2 * (sizeof (mode_t) < sizeof (int)) - 1]; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_promoted_mode_t='int' else gl_cv_promoted_mode_t='mode_t' fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_promoted_mode_t" >&5 $as_echo "$gl_cv_promoted_mode_t" >&6; } cat >>confdefs.h <<_ACEOF #define PROMOTED_MODE_T $gl_cv_promoted_mode_t _ACEOF ac_fn_c_check_decl "$LINENO" "setenv" "ac_cv_have_decl_setenv" "$ac_includes_default" if test "x$ac_cv_have_decl_setenv" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_SETENV $ac_have_decl _ACEOF if test $ac_cv_have_decl_setenv = no; then HAVE_DECL_SETENV=0 fi for ac_header in search.h do : ac_fn_c_check_header_mongrel "$LINENO" "search.h" "ac_cv_header_search_h" "$ac_includes_default" if test "x$ac_cv_header_search_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_SEARCH_H 1 _ACEOF fi done for ac_func in tsearch do : ac_fn_c_check_func "$LINENO" "tsearch" "ac_cv_func_tsearch" if test "x$ac_cv_func_tsearch" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_TSEARCH 1 _ACEOF fi done GNULIB_MKTIME=0; GNULIB_NANOSLEEP=0; GNULIB_STRPTIME=0; GNULIB_TIMEGM=0; GNULIB_TIME_R=0; GNULIB_TIME_RZ=0; HAVE_DECL_LOCALTIME_R=1; HAVE_NANOSLEEP=1; HAVE_STRPTIME=1; HAVE_TIMEGM=1; REPLACE_LOCALTIME_R=GNULIB_PORTCHECK; REPLACE_MKTIME=GNULIB_PORTCHECK; REPLACE_NANOSLEEP=GNULIB_PORTCHECK; REPLACE_TIMEGM=GNULIB_PORTCHECK; : ${GNULIB_GETTIMEOFDAY=0}; REPLACE_GMTIME=0; REPLACE_LOCALTIME=0; { $as_echo "$as_me:${as_lineno-$LINENO}: checking for struct timespec in " >&5 $as_echo_n "checking for struct timespec in ... " >&6; } if ${gl_cv_sys_struct_timespec_in_time_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { static struct timespec x; x.tv_sec = x.tv_nsec; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_sys_struct_timespec_in_time_h=yes else gl_cv_sys_struct_timespec_in_time_h=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_sys_struct_timespec_in_time_h" >&5 $as_echo "$gl_cv_sys_struct_timespec_in_time_h" >&6; } TIME_H_DEFINES_STRUCT_TIMESPEC=0 SYS_TIME_H_DEFINES_STRUCT_TIMESPEC=0 PTHREAD_H_DEFINES_STRUCT_TIMESPEC=0 UNISTD_H_DEFINES_STRUCT_TIMESPEC=0 if test $gl_cv_sys_struct_timespec_in_time_h = yes; then TIME_H_DEFINES_STRUCT_TIMESPEC=1 else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for struct timespec in " >&5 $as_echo_n "checking for struct timespec in ... " >&6; } if ${gl_cv_sys_struct_timespec_in_sys_time_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { static struct timespec x; x.tv_sec = x.tv_nsec; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_sys_struct_timespec_in_sys_time_h=yes else gl_cv_sys_struct_timespec_in_sys_time_h=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_sys_struct_timespec_in_sys_time_h" >&5 $as_echo "$gl_cv_sys_struct_timespec_in_sys_time_h" >&6; } if test $gl_cv_sys_struct_timespec_in_sys_time_h = yes; then SYS_TIME_H_DEFINES_STRUCT_TIMESPEC=1 else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for struct timespec in " >&5 $as_echo_n "checking for struct timespec in ... 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BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_FR") != NULL) { if (btowc (EOF) != WEOF) return 1; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_btowc_eof=yes else gl_cv_func_btowc_eof=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_btowc_eof" >&5 $as_echo "$gl_cv_func_btowc_eof" >&6; } case "$gl_cv_func_btowc_nul" in *yes) ;; *) REPLACE_BTOWC=1 ;; esac case "$gl_cv_func_btowc_eof" in *yes) ;; *) REPLACE_BTOWC=1 ;; esac fi if test $HAVE_BTOWC = 0 || test $REPLACE_BTOWC = 1; then gl_LIBOBJS="$gl_LIBOBJS btowc.$ac_objext" : fi GNULIB_BTOWC=1 $as_echo "#define GNULIB_TEST_BTOWC 1" >>confdefs.h if test "x$datarootdir" = x; then datarootdir='${datadir}' fi if test "x$docdir" = x; then docdir='${datarootdir}/doc/${PACKAGE_TARNAME}' fi if test "x$htmldir" = x; then htmldir='${docdir}' fi if test "x$dvidir" = x; then dvidir='${docdir}' fi if test "x$pdfdir" = x; then pdfdir='${docdir}' fi if test "x$psdir" = x; then psdir='${docdir}' fi if test "x$lispdir" = x; then lispdir='${datarootdir}/emacs/site-lisp' fi if test "x$localedir" = x; then localedir='${datarootdir}/locale' fi if test "x$runstatedir" = x; then runstatedir='${localstatedir}/run' fi pkglibexecdir='${libexecdir}/${PACKAGE}' { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether // is distinct from /" >&5 $as_echo_n "checking whether // is distinct from /... 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" >&6; } if ${gl_cv_next_float_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'float.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_float_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_float_h gl_cv_next_float_h='"'$gl_header'"' fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_float_h" >&5 $as_echo "$gl_cv_next_float_h" >&6; } fi NEXT_FLOAT_H=$gl_cv_next_float_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'float.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_float_h fi NEXT_AS_FIRST_DIRECTIVE_FLOAT_H=$gl_next_as_first_directive fi if test -n "$FLOAT_H"; then GL_GENERATE_FLOAT_H_TRUE= GL_GENERATE_FLOAT_H_FALSE='#' else GL_GENERATE_FLOAT_H_TRUE='#' GL_GENERATE_FLOAT_H_FALSE= fi if test $REPLACE_FLOAT_LDBL = 1; then gl_LIBOBJS="$gl_LIBOBJS float.$ac_objext" fi if test $REPLACE_ITOLD = 1; then gl_LIBOBJS="$gl_LIBOBJS itold.$ac_objext" fi if test $REPLACE_GETOPT = 1; then gl_LIBOBJS="$gl_LIBOBJS getopt.$ac_objext" gl_LIBOBJS="$gl_LIBOBJS getopt1.$ac_objext" GNULIB_GL_UNISTD_H_GETOPT=1 fi $as_echo "#define GNULIB_TEST_GETOPT_GNU 1" >>confdefs.h REPLACE_GETOPT=1 if test $REPLACE_GETOPT = 1; then GETOPT_H=getopt.h $as_echo "#define __GETOPT_PREFIX rpl_" >>confdefs.h fi if test $REPLACE_GETOPT = 1; then gl_LIBOBJS="$gl_LIBOBJS getopt.$ac_objext" gl_LIBOBJS="$gl_LIBOBJS getopt1.$ac_objext" GNULIB_GL_UNISTD_H_GETOPT=1 fi ac_found=0 ac_fn_c_check_decl "$LINENO" "program_invocation_name" "ac_cv_have_decl_program_invocation_name" "#include " if test "x$ac_cv_have_decl_program_invocation_name" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_PROGRAM_INVOCATION_NAME $ac_have_decl _ACEOF if test $ac_have_decl = 1; then : ac_found=1 fi ac_fn_c_check_decl "$LINENO" "program_invocation_short_name" "ac_cv_have_decl_program_invocation_short_name" "#include " if test "x$ac_cv_have_decl_program_invocation_short_name" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME $ac_have_decl _ACEOF if test $ac_have_decl = 1; then : ac_found=1 fi ac_fn_c_check_decl "$LINENO" "__argv" "ac_cv_have_decl___argv" "#include " if test "x$ac_cv_have_decl___argv" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL___ARGV $ac_have_decl _ACEOF if test $ac_have_decl = 1; then : ac_found=1 fi # Incur the cost of this test only if none of the above worked. if test $ac_found = 0; then # On OpenBSD 5.1, using the global __progname variable appears to be # the only way to implement getprogname. { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether __progname is defined in default libraries" >&5 $as_echo_n "checking whether __progname is defined in default libraries... 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" >&6; } if ${gl_cv_next_langinfo_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_langinfo_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'langinfo.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_langinfo_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_langinfo_h gl_cv_next_langinfo_h='"'$gl_header'"' else gl_cv_next_langinfo_h='<'langinfo.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_langinfo_h" >&5 $as_echo "$gl_cv_next_langinfo_h" >&6; } fi NEXT_LANGINFO_H=$gl_cv_next_langinfo_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'langinfo.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_langinfo_h fi NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H=$gl_next_as_first_directive HAVE_LANGINFO_CODESET=0 HAVE_LANGINFO_T_FMT_AMPM=0 HAVE_LANGINFO_ERA=0 HAVE_LANGINFO_YESEXPR=0 if test $ac_cv_header_langinfo_h = yes; then HAVE_LANGINFO_H=1 { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether langinfo.h defines CODESET" >&5 $as_echo_n "checking whether langinfo.h defines CODESET... " >&6; } if ${gl_cv_header_langinfo_codeset+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int a = CODESET; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_langinfo_codeset=yes else gl_cv_header_langinfo_codeset=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_langinfo_codeset" >&5 $as_echo "$gl_cv_header_langinfo_codeset" >&6; } if test $gl_cv_header_langinfo_codeset = yes; then HAVE_LANGINFO_CODESET=1 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether langinfo.h defines T_FMT_AMPM" >&5 $as_echo_n "checking whether langinfo.h defines T_FMT_AMPM... " >&6; } if ${gl_cv_header_langinfo_t_fmt_ampm+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int a = T_FMT_AMPM; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_langinfo_t_fmt_ampm=yes else gl_cv_header_langinfo_t_fmt_ampm=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_langinfo_t_fmt_ampm" >&5 $as_echo "$gl_cv_header_langinfo_t_fmt_ampm" >&6; } if test $gl_cv_header_langinfo_t_fmt_ampm = yes; then HAVE_LANGINFO_T_FMT_AMPM=1 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether langinfo.h defines ERA" >&5 $as_echo_n "checking whether langinfo.h defines ERA... " >&6; } if ${gl_cv_header_langinfo_era+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int a = ERA; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_langinfo_era=yes else gl_cv_header_langinfo_era=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_langinfo_era" >&5 $as_echo "$gl_cv_header_langinfo_era" >&6; } if test $gl_cv_header_langinfo_era = yes; then HAVE_LANGINFO_ERA=1 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether langinfo.h defines YESEXPR" >&5 $as_echo_n "checking whether langinfo.h defines YESEXPR... " >&6; } if ${gl_cv_header_langinfo_yesexpr+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int a = YESEXPR; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_langinfo_yesexpr=yes else gl_cv_header_langinfo_yesexpr=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_langinfo_yesexpr" >&5 $as_echo "$gl_cv_header_langinfo_yesexpr" >&6; } if test $gl_cv_header_langinfo_yesexpr = yes; then HAVE_LANGINFO_YESEXPR=1 fi else HAVE_LANGINFO_H=0 fi for gl_func in nl_langinfo; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done LOCALCHARSET_TESTS_ENVIRONMENT="CHARSETALIASDIR=\"\$(abs_top_builddir)/$gl_source_base\"" case "$host_os" in solaris*) $as_echo "#define _LCONV_C99 1" >>confdefs.h ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether locale.h conforms to POSIX:2001" >&5 $as_echo_n "checking whether locale.h conforms to POSIX:2001... " >&6; } if ${gl_cv_header_locale_h_posix2001+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int x = LC_MESSAGES; int y = sizeof (((struct lconv *) 0)->decimal_point); int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_locale_h_posix2001=yes else gl_cv_header_locale_h_posix2001=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_locale_h_posix2001" >&5 $as_echo "$gl_cv_header_locale_h_posix2001" >&6; } if test $ac_cv_header_xlocale_h = yes; then HAVE_XLOCALE_H=1 { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether locale.h defines locale_t" >&5 $as_echo_n "checking whether locale.h defines locale_t... " >&6; } if ${gl_cv_header_locale_has_locale_t+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include locale_t x; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_locale_has_locale_t=yes else gl_cv_header_locale_has_locale_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_locale_has_locale_t" >&5 $as_echo "$gl_cv_header_locale_has_locale_t" >&6; } if test $gl_cv_header_locale_has_locale_t = yes; then gl_cv_header_locale_h_needs_xlocale_h=no else gl_cv_header_locale_h_needs_xlocale_h=yes fi else HAVE_XLOCALE_H=0 gl_cv_header_locale_h_needs_xlocale_h=no fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether struct lconv is properly defined" >&5 $as_echo_n "checking whether struct lconv is properly defined... " >&6; } if ${gl_cv_sys_struct_lconv_ok+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include struct lconv l; int x = sizeof (l.decimal_point); int y = sizeof (l.int_p_cs_precedes); int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_sys_struct_lconv_ok=yes else gl_cv_sys_struct_lconv_ok=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_sys_struct_lconv_ok" >&5 $as_echo "$gl_cv_sys_struct_lconv_ok" >&6; } if test $gl_cv_sys_struct_lconv_ok = no; then REPLACE_STRUCT_LCONV=1 fi if test $gl_cv_have_include_next = yes; then gl_cv_next_locale_h='<'locale.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_locale_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'locale.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_locale_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_locale_h gl_cv_next_locale_h='"'$gl_header'"' fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_locale_h" >&5 $as_echo "$gl_cv_next_locale_h" >&6; } fi NEXT_LOCALE_H=$gl_cv_next_locale_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'locale.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_locale_h fi NEXT_AS_FIRST_DIRECTIVE_LOCALE_H=$gl_next_as_first_directive for gl_func in setlocale duplocale; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include /* Some systems provide declarations in a non-standard header. */ #if HAVE_XLOCALE_H # include #endif int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done if test $REPLACE_STRUCT_LCONV = 1; then REPLACE_LOCALECONV=1 fi if test $REPLACE_LOCALECONV = 1; then gl_LIBOBJS="$gl_LIBOBJS localeconv.$ac_objext" ac_fn_c_check_member "$LINENO" "struct lconv" "decimal_point" "ac_cv_member_struct_lconv_decimal_point" "#include " if test "x$ac_cv_member_struct_lconv_decimal_point" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STRUCT_LCONV_DECIMAL_POINT 1 _ACEOF fi fi GNULIB_LOCALECONV=1 $as_echo "#define GNULIB_TEST_LOCALECONV 1" >>confdefs.h if test "$gl_threads_api" = posix; then # OSF/1 4.0 and Mac OS X 10.1 lack the pthread_rwlock_t type and the # pthread_rwlock_* functions. ac_fn_c_check_type "$LINENO" "pthread_rwlock_t" "ac_cv_type_pthread_rwlock_t" "#include " if test "x$ac_cv_type_pthread_rwlock_t" = xyes; then : $as_echo "#define HAVE_PTHREAD_RWLOCK 1" >>confdefs.h fi # glibc defines PTHREAD_MUTEX_RECURSIVE as enum, not as a macro. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #if __FreeBSD__ == 4 error "No, in FreeBSD 4.0 recursive mutexes actually don't work." #elif (defined __ENVIRONMENT_MAC_OS_X_VERSION_MIN_REQUIRED__ \ && __ENVIRONMENT_MAC_OS_X_VERSION_MIN_REQUIRED__ < 1070) error "No, in Mac OS X < 10.7 recursive mutexes actually don't work." #else int x = (int)PTHREAD_MUTEX_RECURSIVE; return !x; #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : $as_echo "#define HAVE_PTHREAD_MUTEX_RECURSIVE 1" >>confdefs.h fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi : cat >>confdefs.h <<_ACEOF #define GNULIB_LOCK 1 _ACEOF for ac_header in stdlib.h do : ac_fn_c_check_header_mongrel "$LINENO" "stdlib.h" "ac_cv_header_stdlib_h" "$ac_includes_default" if test "x$ac_cv_header_stdlib_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STDLIB_H 1 _ACEOF fi done { $as_echo "$as_me:${as_lineno-$LINENO}: checking for GNU libc compatible malloc" >&5 $as_echo_n "checking for GNU libc compatible malloc... " >&6; } if ${ac_cv_func_malloc_0_nonnull+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on platforms where we know the result. *-gnu* | freebsd* | netbsd* | openbsd* \ | hpux* | solaris* | cygwin* | mingw*) ac_cv_func_malloc_0_nonnull=yes ;; # If we don't know, assume the worst. *) ac_cv_func_malloc_0_nonnull=no ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if defined STDC_HEADERS || defined HAVE_STDLIB_H # include #else char *malloc (); #endif int main () { char *p = malloc (0); int result = !p; free (p); return result; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : ac_cv_func_malloc_0_nonnull=yes else ac_cv_func_malloc_0_nonnull=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_func_malloc_0_nonnull" >&5 $as_echo "$ac_cv_func_malloc_0_nonnull" >&6; } if test $ac_cv_func_malloc_0_nonnull = yes; then : $as_echo "#define HAVE_MALLOC_GNU 1" >>confdefs.h else $as_echo "#define HAVE_MALLOC_GNU 0" >>confdefs.h REPLACE_MALLOC=1 fi if test $REPLACE_MALLOC = 1; then gl_LIBOBJS="$gl_LIBOBJS malloc.$ac_objext" fi cat >>confdefs.h <<_ACEOF #define GNULIB_MALLOC_GNU 1 _ACEOF if test $gl_cv_func_malloc_posix = yes; then $as_echo "#define HAVE_MALLOC_POSIX 1" >>confdefs.h else REPLACE_MALLOC=1 fi if test $REPLACE_MALLOC = 1; then gl_LIBOBJS="$gl_LIBOBJS malloc.$ac_objext" fi GNULIB_MALLOC_POSIX=1 $as_echo "#define GNULIB_TEST_MALLOC_POSIX 1" >>confdefs.h if test $gl_cv_have_include_next = yes; then gl_cv_next_math_h='<'math.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_math_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_math_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'math.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_math_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_math_h gl_cv_next_math_h='"'$gl_header'"' else gl_cv_next_math_h='<'math.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_math_h" >&5 $as_echo "$gl_cv_next_math_h" >&6; } fi NEXT_MATH_H=$gl_cv_next_math_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'math.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_math_h fi NEXT_AS_FIRST_DIRECTIVE_MATH_H=$gl_next_as_first_directive { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether NAN macro works" >&5 $as_echo_n "checking whether NAN macro works... " >&6; } if ${gl_cv_header_math_nan_works+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { /* Solaris 10 has a broken definition of NAN. Other platforms fail to provide NAN, or provide it only in C99 mode; this test only needs to fail when NAN is provided but wrong. */ float f = 1.0f; #ifdef NAN f = NAN; #endif return f == 0; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_math_nan_works=yes else gl_cv_header_math_nan_works=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_math_nan_works" >&5 $as_echo "$gl_cv_header_math_nan_works" >&6; } if test $gl_cv_header_math_nan_works = no; then REPLACE_NAN=1 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether HUGE_VAL works" >&5 $as_echo_n "checking whether HUGE_VAL works... " >&6; } if ${gl_cv_header_math_huge_val_works+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { /* Solaris 10 has a broken definition of HUGE_VAL. */ double d = HUGE_VAL; return d == 0; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_math_huge_val_works=yes else gl_cv_header_math_huge_val_works=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_math_huge_val_works" >&5 $as_echo "$gl_cv_header_math_huge_val_works" >&6; } if test $gl_cv_header_math_huge_val_works = no; then REPLACE_HUGE_VAL=1 fi for gl_func in acosf acosl asinf asinl atanf atanl cbrt cbrtf cbrtl ceilf ceill copysign copysignf copysignl cosf cosl coshf expf expl exp2 exp2f exp2l expm1 expm1f expm1l fabsf fabsl floorf floorl fma fmaf fmal fmod fmodf fmodl frexpf frexpl hypotf hypotl ilogb ilogbf ilogbl ldexpf ldexpl log logf logl log10 log10f log10l log1p log1pf log1pl log2 log2f log2l logb logbf logbl modf modff modfl powf remainder remainderf remainderl rint rintf rintl round roundf roundl sinf sinl sinhf sqrtf sqrtl tanf tanl tanhf trunc truncf truncl; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... 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" >&6; } if ${gl_cv_func_mbrtowc_incomplete_state+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on AIX and OSF/1. aix* | osf*) gl_cv_func_mbrtowc_incomplete_state="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_incomplete_state="guessing yes" ;; esac if test $LOCALE_JA != none; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { const char input[] = "B\217\253\344\217\251\316er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) if (mbsinit (&state)) return 1; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_incomplete_state=yes else gl_cv_func_mbrtowc_incomplete_state=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_incomplete_state" >&5 $as_echo "$gl_cv_func_mbrtowc_incomplete_state" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc works as well as mbtowc" >&5 $as_echo_n "checking whether mbrtowc works as well as mbtowc... " >&6; } if ${gl_cv_func_mbrtowc_sanitycheck+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on Solaris 8. solaris2.8) gl_cv_func_mbrtowc_sanitycheck="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_sanitycheck="guessing yes" ;; esac if test $LOCALE_ZH_CN != none; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { /* This fails on Solaris 8: mbrtowc returns 2, and sets wc to 0x00F0. mbtowc returns 4 (correct) and sets wc to 0x5EDC. */ if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { char input[] = "B\250\271\201\060\211\070er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 6, &state) != 4 && mbtowc (&wc, input + 3, 6) == 4) return 1; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_sanitycheck=yes else gl_cv_func_mbrtowc_sanitycheck=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_sanitycheck" >&5 $as_echo "$gl_cv_func_mbrtowc_sanitycheck" >&6; } REPLACE_MBSTATE_T=0 case "$gl_cv_func_mbrtowc_incomplete_state" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac case "$gl_cv_func_mbrtowc_sanitycheck" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac else REPLACE_MBSTATE_T=1 fi if test $ac_cv_func_mbrtowc = no; then HAVE_MBRTOWC=0 ac_fn_c_check_decl "$LINENO" "mbrtowc" "ac_cv_have_decl_mbrtowc" " /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include " if test "x$ac_cv_have_decl_mbrtowc" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_MBRTOWC $ac_have_decl _ACEOF if test $ac_cv_have_decl_mbrtowc = yes; then REPLACE_MBRTOWC=1 fi else if test $REPLACE_MBSTATE_T = 1; then REPLACE_MBRTOWC=1 else { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc handles a NULL pwc argument" >&5 $as_echo_n "checking whether mbrtowc handles a NULL pwc argument... 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BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { int result = 0; if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { char input[] = "\303\237er"; mbstate_t state; wchar_t wc; size_t ret; memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 5, &state); if (ret != 2) result |= 1; if (!mbsinit (&state)) result |= 2; memset (&state, '\0', sizeof (mbstate_t)); ret = mbrtowc (NULL, input, 5, &state); if (ret != 2) /* Solaris 7 fails here: ret is -1. */ result |= 4; if (!mbsinit (&state)) result |= 8; } return result; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_null_arg1=yes else gl_cv_func_mbrtowc_null_arg1=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_null_arg1" >&5 $as_echo "$gl_cv_func_mbrtowc_null_arg1" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc handles a NULL string argument" >&5 $as_echo_n "checking whether mbrtowc handles a NULL string argument... " >&6; } if ${gl_cv_func_mbrtowc_null_arg2+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on OSF/1. osf*) gl_cv_func_mbrtowc_null_arg2="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_null_arg2="guessing yes" ;; esac if test $LOCALE_FR_UTF8 != none; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { mbstate_t state; wchar_t wc; int ret; memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; mbrtowc (&wc, NULL, 5, &state); /* Check that wc was not modified. */ if (wc != (wchar_t) 0xBADFACE) return 1; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_null_arg2=yes else gl_cv_func_mbrtowc_null_arg2=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_null_arg2" >&5 $as_echo "$gl_cv_func_mbrtowc_null_arg2" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc has a correct return value" >&5 $as_echo_n "checking whether mbrtowc has a correct return value... " >&6; } if ${gl_cv_func_mbrtowc_retval+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on HP-UX, Solaris, native Windows. hpux* | solaris* | mingw*) gl_cv_func_mbrtowc_retval="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_retval="guessing yes" ;; esac if test $LOCALE_FR_UTF8 != none || test $LOCALE_JA != none \ || { case "$host_os" in mingw*) true;; *) false;; esac; }; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { int result = 0; int found_some_locale = 0; /* This fails on Solaris. */ if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { char input[] = "B\303\274\303\237er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) { input[1] = '\0'; if (mbrtowc (&wc, input + 2, 5, &state) != 1) result |= 1; } found_some_locale = 1; } /* This fails on HP-UX 11.11. */ if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { char input[] = "B\217\253\344\217\251\316er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) { input[1] = '\0'; if (mbrtowc (&wc, input + 2, 5, &state) != 2) result |= 2; } found_some_locale = 1; } /* This fails on native Windows. */ if (setlocale (LC_ALL, "Japanese_Japan.932") != NULL) { char input[] = "<\223\372\226\173\214\352>"; /* "<日本語>" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 1, &state) == (size_t)(-2)) { input[3] = '\0'; if (mbrtowc (&wc, input + 4, 4, &state) != 1) result |= 4; } found_some_locale = 1; } if (setlocale (LC_ALL, "Chinese_Taiwan.950") != NULL) { char input[] = "<\244\351\245\273\273\171>"; /* "<日本語>" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 1, &state) == (size_t)(-2)) { input[3] = '\0'; if (mbrtowc (&wc, input + 4, 4, &state) != 1) result |= 8; } found_some_locale = 1; } if (setlocale (LC_ALL, "Chinese_China.936") != NULL) { char input[] = "<\310\325\261\276\325\132>"; /* "<日本語>" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 1, &state) == (size_t)(-2)) { input[3] = '\0'; if (mbrtowc (&wc, input + 4, 4, &state) != 1) result |= 16; } found_some_locale = 1; } return (found_some_locale ? result : 77); } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_retval=yes else if test $? != 77; then gl_cv_func_mbrtowc_retval=no fi fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_retval" >&5 $as_echo "$gl_cv_func_mbrtowc_retval" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc returns 0 when parsing a NUL character" >&5 $as_echo_n "checking whether mbrtowc returns 0 when parsing a NUL character... " >&6; } if ${gl_cv_func_mbrtowc_nul_retval+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on Solaris 8 and 9. solaris2.[89]) gl_cv_func_mbrtowc_nul_retval="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_nul_retval="guessing yes" ;; esac if test $LOCALE_ZH_CN != none; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { /* This fails on Solaris 8 and 9. */ if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, "", 1, &state) != 0) return 1; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_nul_retval=yes else gl_cv_func_mbrtowc_nul_retval=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_nul_retval" >&5 $as_echo "$gl_cv_func_mbrtowc_nul_retval" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc works on empty input" >&5 $as_echo_n "checking whether mbrtowc works on empty input... " >&6; } if ${gl_cv_func_mbrtowc_empty_input+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on AIX and glibc systems. aix* | *-gnu*) gl_cv_func_mbrtowc_empty_input="guessing no" ;; *) gl_cv_func_mbrtowc_empty_input="guessing yes" ;; esac if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include static wchar_t wc; static mbstate_t mbs; int main (void) { return mbrtowc (&wc, "", 0, &mbs) != (size_t) -2; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_empty_input=yes else gl_cv_func_mbrtowc_empty_input=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_empty_input" >&5 $as_echo "$gl_cv_func_mbrtowc_empty_input" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether the C locale is free of encoding errors" >&5 $as_echo_n "checking whether the C locale is free of encoding errors... " >&6; } if ${gl_cv_C_locale_sans_EILSEQ+:} false; then : $as_echo_n "(cached) " >&6 else gl_cv_C_locale_sans_EILSEQ="guessing no" if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include int main () { int i; char *locale = setlocale (LC_ALL, "C"); if (! locale) return 1; for (i = CHAR_MIN; i <= CHAR_MAX; i++) { char c = i; wchar_t wc; mbstate_t mbs = { 0, }; size_t ss = mbrtowc (&wc, &c, 1, &mbs); if (1 < ss) return 1; } return 0; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_C_locale_sans_EILSEQ=yes else gl_cv_C_locale_sans_EILSEQ=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_C_locale_sans_EILSEQ" >&5 $as_echo "$gl_cv_C_locale_sans_EILSEQ" >&6; } case "$gl_cv_func_mbrtowc_null_arg1" in *yes) ;; *) $as_echo "#define MBRTOWC_NULL_ARG1_BUG 1" >>confdefs.h REPLACE_MBRTOWC=1 ;; esac case "$gl_cv_func_mbrtowc_null_arg2" in *yes) ;; *) $as_echo "#define MBRTOWC_NULL_ARG2_BUG 1" >>confdefs.h REPLACE_MBRTOWC=1 ;; esac case "$gl_cv_func_mbrtowc_retval" in *yes) ;; *) $as_echo "#define MBRTOWC_RETVAL_BUG 1" >>confdefs.h REPLACE_MBRTOWC=1 ;; esac case "$gl_cv_func_mbrtowc_nul_retval" in *yes) ;; *) $as_echo "#define MBRTOWC_NUL_RETVAL_BUG 1" >>confdefs.h REPLACE_MBRTOWC=1 ;; esac case "$gl_cv_func_mbrtowc_empty_input" in *yes) ;; *) $as_echo "#define MBRTOWC_EMPTY_INPUT_BUG 1" >>confdefs.h REPLACE_MBRTOWC=1 ;; esac case $gl_cv_C_locale_sans_EILSEQ in *yes) ;; *) $as_echo "#define C_LOCALE_MAYBE_EILSEQ 1" >>confdefs.h REPLACE_MBRTOWC=1 ;; esac fi fi if test $HAVE_MBRTOWC = 0 || test $REPLACE_MBRTOWC = 1; then gl_LIBOBJS="$gl_LIBOBJS mbrtowc.$ac_objext" : fi GNULIB_MBRTOWC=1 $as_echo "#define GNULIB_TEST_MBRTOWC 1" >>confdefs.h if test $ac_cv_func_mbsinit = yes && test $ac_cv_func_mbrtowc = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc handles incomplete characters" >&5 $as_echo_n "checking whether mbrtowc handles incomplete characters... 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BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { const char input[] = "B\217\253\344\217\251\316er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) if (mbsinit (&state)) return 1; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_incomplete_state=yes else gl_cv_func_mbrtowc_incomplete_state=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_incomplete_state" >&5 $as_echo "$gl_cv_func_mbrtowc_incomplete_state" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc works as well as mbtowc" >&5 $as_echo_n "checking whether mbrtowc works as well as mbtowc... " >&6; } if ${gl_cv_func_mbrtowc_sanitycheck+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on Solaris 8. solaris2.8) gl_cv_func_mbrtowc_sanitycheck="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_sanitycheck="guessing yes" ;; esac if test $LOCALE_ZH_CN != none; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { /* This fails on Solaris 8: mbrtowc returns 2, and sets wc to 0x00F0. mbtowc returns 4 (correct) and sets wc to 0x5EDC. */ if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { char input[] = "B\250\271\201\060\211\070er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 6, &state) != 4 && mbtowc (&wc, input + 3, 6) == 4) return 1; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_sanitycheck=yes else gl_cv_func_mbrtowc_sanitycheck=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_sanitycheck" >&5 $as_echo "$gl_cv_func_mbrtowc_sanitycheck" >&6; } REPLACE_MBSTATE_T=0 case "$gl_cv_func_mbrtowc_incomplete_state" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac case "$gl_cv_func_mbrtowc_sanitycheck" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac else REPLACE_MBSTATE_T=1 fi if test $ac_cv_func_mbsinit = no; then HAVE_MBSINIT=0 ac_fn_c_check_decl "$LINENO" "mbsinit" "ac_cv_have_decl_mbsinit" " /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include " if test "x$ac_cv_have_decl_mbsinit" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_MBSINIT $ac_have_decl _ACEOF if test $ac_cv_have_decl_mbsinit = yes; then REPLACE_MBSINIT=1 fi else if test $REPLACE_MBSTATE_T = 1; then REPLACE_MBSINIT=1 else case "$host_os" in mingw*) REPLACE_MBSINIT=1 ;; esac fi fi if test $HAVE_MBSINIT = 0 || test $REPLACE_MBSINIT = 1; then gl_LIBOBJS="$gl_LIBOBJS mbsinit.$ac_objext" : fi GNULIB_MBSINIT=1 $as_echo "#define GNULIB_TEST_MBSINIT 1" >>confdefs.h if false; then REPLACE_MBTOWC=1 fi if test $REPLACE_MBTOWC = 1; then gl_LIBOBJS="$gl_LIBOBJS mbtowc.$ac_objext" : fi GNULIB_MBTOWC=1 $as_echo "#define GNULIB_TEST_MBTOWC 1" >>confdefs.h if test $HAVE_MEMCHR = 0 || test $REPLACE_MEMCHR = 1; then gl_LIBOBJS="$gl_LIBOBJS memchr.$ac_objext" for ac_header in bp-sym.h do : ac_fn_c_check_header_mongrel "$LINENO" "bp-sym.h" "ac_cv_header_bp_sym_h" "$ac_includes_default" if test "x$ac_cv_header_bp_sym_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_BP_SYM_H 1 _ACEOF fi done fi GNULIB_MEMCHR=1 $as_echo "#define GNULIB_TEST_MEMCHR 1" >>confdefs.h for ac_func in mempcpy do : ac_fn_c_check_func "$LINENO" "mempcpy" "ac_cv_func_mempcpy" if test "x$ac_cv_func_mempcpy" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_MEMPCPY 1 _ACEOF fi done if test $ac_cv_func_mempcpy = no; then HAVE_MEMPCPY=0 fi if test $HAVE_MEMPCPY = 0; then gl_LIBOBJS="$gl_LIBOBJS mempcpy.$ac_objext" : fi GNULIB_MEMPCPY=1 $as_echo "#define GNULIB_TEST_MEMPCPY 1" >>confdefs.h if test $HAVE_MSVC_INVALID_PARAMETER_HANDLER = 1; then gl_LIBOBJS="$gl_LIBOBJS msvc-inval.$ac_objext" fi if test $HAVE_MSVC_INVALID_PARAMETER_HANDLER = 1; then gl_LIBOBJS="$gl_LIBOBJS msvc-nothrow.$ac_objext" fi if test $ac_cv_func_nl_langinfo = yes; then # On Irix 6.5, YESEXPR is defined, but nl_langinfo(YESEXPR) is broken. { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether YESEXPR works" >&5 $as_echo_n "checking whether YESEXPR works... " >&6; } if ${gl_cv_func_nl_langinfo_yesexpr_works+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess no on irix systems. irix*) gl_cv_func_nl_langinfo_yesexpr_works="guessing no";; # Guess yes elsewhere. *) gl_cv_func_nl_langinfo_yesexpr_works="guessing yes";; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { return !*nl_langinfo(YESEXPR); ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_nl_langinfo_yesexpr_works=yes else gl_cv_func_nl_langinfo_yesexpr_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_nl_langinfo_yesexpr_works" >&5 $as_echo "$gl_cv_func_nl_langinfo_yesexpr_works" >&6; } case $gl_cv_func_nl_langinfo_yesexpr_works in *yes) FUNC_NL_LANGINFO_YESEXPR_WORKS=1 ;; *) FUNC_NL_LANGINFO_YESEXPR_WORKS=0 ;; esac cat >>confdefs.h <<_ACEOF #define FUNC_NL_LANGINFO_YESEXPR_WORKS $FUNC_NL_LANGINFO_YESEXPR_WORKS _ACEOF if test $HAVE_LANGINFO_CODESET = 1 && test $HAVE_LANGINFO_ERA = 1 \ && test $FUNC_NL_LANGINFO_YESEXPR_WORKS = 1; then : else REPLACE_NL_LANGINFO=1 $as_echo "#define REPLACE_NL_LANGINFO 1" >>confdefs.h fi else HAVE_NL_LANGINFO=0 fi if test $HAVE_NL_LANGINFO = 0 || test $REPLACE_NL_LANGINFO = 1; then gl_LIBOBJS="$gl_LIBOBJS nl_langinfo.$ac_objext" fi GNULIB_NL_LANGINFO=1 $as_echo "#define GNULIB_TEST_NL_LANGINFO 1" >>confdefs.h for ac_header in sys/pstat.h sys/sysmp.h sys/param.h do : as_ac_Header=`$as_echo "ac_cv_header_$ac_header" | $as_tr_sh` ac_fn_c_check_header_compile "$LINENO" "$ac_header" "$as_ac_Header" "$ac_includes_default " if eval test \"x\$"$as_ac_Header"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_$ac_header" | $as_tr_cpp` 1 _ACEOF fi done for ac_header in sys/sysctl.h do : ac_fn_c_check_header_compile "$LINENO" "sys/sysctl.h" "ac_cv_header_sys_sysctl_h" "$ac_includes_default #if HAVE_SYS_PARAM_H # include #endif " if test "x$ac_cv_header_sys_sysctl_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_SYS_SYSCTL_H 1 _ACEOF fi done for ac_func in sched_getaffinity sched_getaffinity_np \ pstat_getdynamic sysmp sysctl do : as_ac_var=`$as_echo "ac_cv_func_$ac_func" | $as_tr_sh` ac_fn_c_check_func "$LINENO" "$ac_func" "$as_ac_var" if eval test \"x\$"$as_ac_var"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_$ac_func" | $as_tr_cpp` 1 _ACEOF fi done if test $ac_cv_func_sched_getaffinity = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking for glibc compatible sched_getaffinity" >&5 $as_echo_n "checking for glibc compatible sched_getaffinity... 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" >&6; } if ${gl_cv_func_re_compile_pattern_working+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : gl_cv_func_re_compile_pattern_working=no else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #include #if defined M_CHECK_ACTION || HAVE_DECL_ALARM # include # include #endif #if HAVE_MALLOC_H # include #endif #ifdef M_CHECK_ACTION /* Exit with distinguishable exit code. */ static void sigabrt_no_core (int sig) { raise (SIGTERM); } #endif int main () { int result = 0; static struct re_pattern_buffer regex; unsigned char folded_chars[UCHAR_MAX + 1]; int i; const char *s; struct re_registers regs; /* Some builds of glibc go into an infinite loop on this test. Use alarm to force death, and mallopt to avoid malloc recursion in diagnosing the corrupted heap. */ #if HAVE_DECL_ALARM signal (SIGALRM, SIG_DFL); alarm (2); #endif #ifdef M_CHECK_ACTION signal (SIGABRT, sigabrt_no_core); mallopt (M_CHECK_ACTION, 2); #endif if (setlocale (LC_ALL, "en_US.UTF-8")) { { /* http://sourceware.org/ml/libc-hacker/2006-09/msg00008.html This test needs valgrind to catch the bug on Debian GNU/Linux 3.1 x86, but it might catch the bug better on other platforms and it shouldn't hurt to try the test here. */ static char const pat[] = "insert into"; static char const data[] = "\xFF\0\x12\xA2\xAA\xC4\xB1,K\x12\xC4\xB1*\xACK"; re_set_syntax (RE_SYNTAX_GREP | RE_HAT_LISTS_NOT_NEWLINE | RE_ICASE); memset (®ex, 0, sizeof regex); s = re_compile_pattern (pat, sizeof pat - 1, ®ex); if (s) result |= 1; else if (re_search (®ex, data, sizeof data - 1, 0, sizeof data - 1, ®s) != -1) result |= 1; regfree (®ex); } { /* This test is from glibc bug 15078. The test case is from Andreas Schwab in . */ static char const pat[] = "[^x]x"; static char const data[] = /* */ "\xe1\x80\x80" "\xe1\x80\xbb" "\xe1\x80\xbd" "\xe1\x80\x94" "\xe1\x80\xba" "\xe1\x80\xaf" "\xe1\x80\x95" "\xe1\x80\xba" "x"; re_set_syntax (0); memset (®ex, 0, sizeof regex); s = re_compile_pattern (pat, sizeof pat - 1, ®ex); if (s) result |= 1; else { i = re_search (®ex, data, sizeof data - 1, 0, sizeof data - 1, 0); if (i != 0 && i != 21) result |= 1; } regfree (®ex); } if (! setlocale (LC_ALL, "C")) return 1; } /* This test is from glibc bug 3957, reported by Andrew Mackey. */ re_set_syntax (RE_SYNTAX_EGREP | RE_HAT_LISTS_NOT_NEWLINE); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("a[^x]b", 6, ®ex); if (s) result |= 2; /* This should fail, but succeeds for glibc-2.5. */ else if (re_search (®ex, "a\nb", 3, 0, 3, ®s) != -1) result |= 2; /* This regular expression is from Spencer ere test number 75 in grep-2.3. */ re_set_syntax (RE_SYNTAX_POSIX_EGREP); memset (®ex, 0, sizeof regex); for (i = 0; i <= UCHAR_MAX; i++) folded_chars[i] = i; regex.translate = folded_chars; s = re_compile_pattern ("a[[:]:]]b\n", 11, ®ex); /* This should fail with _Invalid character class name_ error. */ if (!s) result |= 4; /* Ensure that [b-a] is diagnosed as invalid, when using RE_NO_EMPTY_RANGES. */ re_set_syntax (RE_SYNTAX_POSIX_EGREP | RE_NO_EMPTY_RANGES); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("a[b-a]", 6, ®ex); if (s == 0) result |= 8; /* This should succeed, but does not for glibc-2.1.3. */ memset (®ex, 0, sizeof regex); s = re_compile_pattern ("{1", 2, ®ex); if (s) result |= 8; /* The following example is derived from a problem report against gawk from Jorge Stolfi . */ memset (®ex, 0, sizeof regex); s = re_compile_pattern ("[an\371]*n", 7, ®ex); if (s) result |= 8; /* This should match, but does not for glibc-2.2.1. */ else if (re_match (®ex, "an", 2, 0, ®s) != 2) result |= 8; memset (®ex, 0, sizeof regex); s = re_compile_pattern ("x", 1, ®ex); if (s) result |= 8; /* glibc-2.2.93 does not work with a negative RANGE argument. */ else if (re_search (®ex, "wxy", 3, 2, -2, ®s) != 1) result |= 8; /* The version of regex.c in older versions of gnulib ignored RE_ICASE. Detect that problem too. */ re_set_syntax (RE_SYNTAX_EMACS | RE_ICASE); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("x", 1, ®ex); if (s) result |= 16; else if (re_search (®ex, "WXY", 3, 0, 3, ®s) < 0) result |= 16; /* Catch a bug reported by Vin Shelton in http://lists.gnu.org/archive/html/bug-coreutils/2007-06/msg00089.html */ re_set_syntax (RE_SYNTAX_POSIX_BASIC & ~RE_CONTEXT_INVALID_DUP & ~RE_NO_EMPTY_RANGES); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("[[:alnum:]_-]\\\\+$", 16, ®ex); if (s) result |= 32; /* REG_STARTEND was added to glibc on 2004-01-15. Reject older versions. */ if (! REG_STARTEND) result |= 64; #if 0 /* It would be nice to reject hosts whose regoff_t values are too narrow (including glibc on hosts with 64-bit ptrdiff_t and 32-bit int), but we should wait until glibc implements this feature. Otherwise, support for equivalence classes and multibyte collation symbols would always be broken except when compiling --without-included-regex. */ if (sizeof (regoff_t) < sizeof (ptrdiff_t) || sizeof (regoff_t) < sizeof (ssize_t)) result |= 64; #endif return result; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_re_compile_pattern_working=yes else gl_cv_func_re_compile_pattern_working=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_re_compile_pattern_working" >&5 $as_echo "$gl_cv_func_re_compile_pattern_working" >&6; } case $gl_cv_func_re_compile_pattern_working in #( yes) ac_use_included_regex=no;; #( no) ac_use_included_regex=yes;; esac ;; *) as_fn_error $? "Invalid value for --with-included-regex: $with_included_regex" "$LINENO" 5 ;; esac if test $ac_use_included_regex = yes; then $as_echo "#define _REGEX_INCLUDE_LIMITS_H 1" >>confdefs.h $as_echo "#define _REGEX_LARGE_OFFSETS 1" >>confdefs.h $as_echo "#define re_syntax_options rpl_re_syntax_options" >>confdefs.h $as_echo "#define re_set_syntax rpl_re_set_syntax" >>confdefs.h $as_echo "#define re_compile_pattern rpl_re_compile_pattern" >>confdefs.h $as_echo "#define re_compile_fastmap rpl_re_compile_fastmap" >>confdefs.h $as_echo "#define re_search rpl_re_search" >>confdefs.h $as_echo "#define re_search_2 rpl_re_search_2" >>confdefs.h $as_echo "#define re_match rpl_re_match" >>confdefs.h $as_echo "#define re_match_2 rpl_re_match_2" >>confdefs.h $as_echo "#define re_set_registers rpl_re_set_registers" >>confdefs.h $as_echo "#define re_comp rpl_re_comp" >>confdefs.h $as_echo "#define re_exec rpl_re_exec" >>confdefs.h $as_echo "#define regcomp rpl_regcomp" >>confdefs.h $as_echo "#define regexec rpl_regexec" >>confdefs.h $as_echo "#define regerror rpl_regerror" >>confdefs.h $as_echo "#define regfree rpl_regfree" >>confdefs.h fi if test $ac_use_included_regex = yes; then gl_LIBOBJS="$gl_LIBOBJS regex.$ac_objext" for ac_header in libintl.h do : ac_fn_c_check_header_mongrel "$LINENO" "libintl.h" "ac_cv_header_libintl_h" "$ac_includes_default" if test "x$ac_cv_header_libintl_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_LIBINTL_H 1 _ACEOF fi done ac_fn_c_check_decl "$LINENO" "isblank" "ac_cv_have_decl_isblank" "#include " if test "x$ac_cv_have_decl_isblank" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_ISBLANK $ac_have_decl _ACEOF fi for ac_header in stdint.h do : ac_fn_c_check_header_mongrel "$LINENO" "stdint.h" "ac_cv_header_stdint_h" "$ac_includes_default" if test "x$ac_cv_header_stdint_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STDINT_H 1 _ACEOF fi done { $as_echo "$as_me:${as_lineno-$LINENO}: checking for SIZE_MAX" >&5 $as_echo_n "checking for SIZE_MAX... " >&6; } if ${gl_cv_size_max+:} false; then : $as_echo_n "(cached) " >&6 else gl_cv_size_max= cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #if HAVE_STDINT_H #include #endif #ifdef SIZE_MAX Found it #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "Found it" >/dev/null 2>&1; then : gl_cv_size_max=yes fi rm -f conftest* if test -z "$gl_cv_size_max"; then if ac_fn_c_compute_int "$LINENO" "sizeof (size_t) * CHAR_BIT - 1" "size_t_bits_minus_1" "#include #include "; then : else size_t_bits_minus_1= fi if ac_fn_c_compute_int "$LINENO" "sizeof (size_t) <= sizeof (unsigned int)" "fits_in_uint" "#include "; then : else fits_in_uint= fi if test -n "$size_t_bits_minus_1" && test -n "$fits_in_uint"; then if test $fits_in_uint = 1; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include extern size_t foo; extern unsigned long foo; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : fits_in_uint=0 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi if test $fits_in_uint = 1; then gl_cv_size_max="(((1U << $size_t_bits_minus_1) - 1) * 2 + 1)" else gl_cv_size_max="(((1UL << $size_t_bits_minus_1) - 1) * 2 + 1)" fi else gl_cv_size_max='((size_t)~(size_t)0)' fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_size_max" >&5 $as_echo "$gl_cv_size_max" >&6; } if test "$gl_cv_size_max" != yes; then cat >>confdefs.h <<_ACEOF #define SIZE_MAX $gl_cv_size_max _ACEOF fi ac_fn_c_check_decl "$LINENO" "sleep" "ac_cv_have_decl_sleep" "#include " if test "x$ac_cv_have_decl_sleep" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_SLEEP $ac_have_decl _ACEOF if test $ac_cv_have_decl_sleep != yes; then HAVE_SLEEP=0 else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for working sleep" >&5 $as_echo_n "checking for working sleep... 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This catches GCC bug 52023 . */ #ifdef __cplusplus template struct alignof_helper { char a; t b; }; # define ao(type) offsetof (alignof_helper, b) #else # define ao(type) offsetof (struct { char a; type b; }, b) #endif char test_double[ao (double) % _Alignof (double) == 0 ? 1 : -1]; char test_long[ao (long int) % _Alignof (long int) == 0 ? 1 : -1]; char test_alignof[alignof (double) == _Alignof (double) ? 1 : -1]; /* Test _Alignas only on platforms where gnulib can help. */ #if \ ((defined __cplusplus && 201103 <= __cplusplus) \ || (defined __APPLE__ && defined __MACH__ \ ? 4 < __GNUC__ + (1 <= __GNUC_MINOR__) \ : __GNUC__) \ || __HP_cc || __HP_aCC || __IBMC__ || __IBMCPP__ \ || __ICC || 0x5110 <= __SUNPRO_C \ || 1300 <= _MSC_VER) struct alignas_test { char c; char alignas (8) alignas_8; }; char test_alignas[offsetof (struct alignas_test, alignas_8) == 8 ? 1 : -1]; #endif int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_working_stdalign_h=yes else gl_cv_header_working_stdalign_h=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_working_stdalign_h" >&5 $as_echo "$gl_cv_header_working_stdalign_h" >&6; } if test $gl_cv_header_working_stdalign_h = yes; then STDALIGN_H='' else STDALIGN_H='stdalign.h' fi if test -n "$STDALIGN_H"; then GL_GENERATE_STDALIGN_H_TRUE= GL_GENERATE_STDALIGN_H_FALSE='#' else GL_GENERATE_STDALIGN_H_TRUE='#' GL_GENERATE_STDALIGN_H_FALSE= fi # Define two additional variables used in the Makefile substitution. if test "$ac_cv_header_stdbool_h" = yes; then STDBOOL_H='' else STDBOOL_H='stdbool.h' fi if test -n "$STDBOOL_H"; then GL_GENERATE_STDBOOL_H_TRUE= GL_GENERATE_STDBOOL_H_FALSE='#' else GL_GENERATE_STDBOOL_H_TRUE='#' GL_GENERATE_STDBOOL_H_FALSE= fi if test "$ac_cv_type__Bool" = yes; then HAVE__BOOL=1 else HAVE__BOOL=0 fi STDDEF_H= ac_fn_c_check_type "$LINENO" "max_align_t" "ac_cv_type_max_align_t" "#include " if test "x$ac_cv_type_max_align_t" = xyes; then : else HAVE_MAX_ALIGN_T=0; STDDEF_H=stddef.h fi if test $gt_cv_c_wchar_t = no; then HAVE_WCHAR_T=0 STDDEF_H=stddef.h fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether NULL can be used in arbitrary expressions" >&5 $as_echo_n "checking whether NULL can be used in arbitrary expressions... 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" >&6; } if ${gl_cv_next_stddef_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'stddef.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_stddef_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_stddef_h gl_cv_next_stddef_h='"'$gl_header'"' fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_stddef_h" >&5 $as_echo "$gl_cv_next_stddef_h" >&6; } fi NEXT_STDDEF_H=$gl_cv_next_stddef_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'stddef.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_stddef_h fi NEXT_AS_FIRST_DIRECTIVE_STDDEF_H=$gl_next_as_first_directive fi $as_echo "#define __USE_MINGW_ANSI_STDIO 1" >>confdefs.h if test $gl_cv_have_include_next = yes; then gl_cv_next_stdio_h='<'stdio.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... 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" >&6; } if ${gl_cv_next_unistd_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_unistd_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'unistd.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_unistd_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_unistd_h gl_cv_next_unistd_h='"'$gl_header'"' else gl_cv_next_unistd_h='<'unistd.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_unistd_h" >&5 $as_echo "$gl_cv_next_unistd_h" >&6; } fi NEXT_UNISTD_H=$gl_cv_next_unistd_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'unistd.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_unistd_h fi NEXT_AS_FIRST_DIRECTIVE_UNISTD_H=$gl_next_as_first_directive if test $ac_cv_header_unistd_h = yes; then HAVE_UNISTD_H=1 else HAVE_UNISTD_H=0 fi for gl_func in chdir chown dup dup2 dup3 environ euidaccess faccessat fchdir fchownat fdatasync fsync ftruncate getcwd getdomainname getdtablesize getgroups gethostname getlogin getlogin_r getpagesize getusershell setusershell endusershell group_member isatty lchown link linkat lseek pipe pipe2 pread pwrite readlink readlinkat rmdir sethostname sleep symlink symlinkat ttyname_r unlink unlinkat usleep; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... 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" >&6; } if ${gl_cv_func_snprintf_size1+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : gl_cv_func_snprintf_size1="guessing yes" else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #if HAVE_SNPRINTF # define my_snprintf snprintf #else # include static int my_snprintf (char *buf, int size, const char *format, ...) { va_list args; int ret; va_start (args, format); ret = vsnprintf (buf, size, format, args); va_end (args); return ret; } #endif int main() { static char buf[8] = { 'D', 'E', 'A', 'D', 'B', 'E', 'E', 'F' }; my_snprintf (buf, 1, "%d", 12345); return buf[1] != 'E'; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_snprintf_size1=yes else gl_cv_func_snprintf_size1=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_snprintf_size1" >&5 $as_echo "$gl_cv_func_snprintf_size1" >&6; } case "$gl_cv_func_snprintf_size1" in *yes) case "$gl_cv_func_snprintf_retval_c99" in *yes) { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether printf supports POSIX/XSI format strings with positions" >&5 $as_echo_n "checking whether printf supports POSIX/XSI format strings with positions... " >&6; } if ${gl_cv_func_printf_positions+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in netbsd[1-3]* | netbsdelf[1-3]* | netbsdaout[1-3]* | netbsdcoff[1-3]*) gl_cv_func_printf_positions="guessing no";; beos*) gl_cv_func_printf_positions="guessing no";; mingw* | pw*) gl_cv_func_printf_positions="guessing no";; *) gl_cv_func_printf_positions="guessing yes";; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include /* The string "%2$d %1$d", with dollar characters protected from the shell's dollar expansion (possibly an autoconf bug). */ static char format[] = { '%', '2', '$', 'd', ' ', '%', '1', '$', 'd', '\0' }; static char buf[100]; int main () { sprintf (buf, format, 33, 55); return (strcmp (buf, "55 33") != 0); } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_printf_positions=yes else gl_cv_func_printf_positions=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_printf_positions" >&5 $as_echo "$gl_cv_func_printf_positions" >&6; } case "$gl_cv_func_printf_positions" in *yes) gl_cv_func_vsnprintf_usable=yes ;; esac ;; esac ;; esac fi if test $gl_cv_func_vsnprintf_usable = no; then gl_LIBOBJS="$gl_LIBOBJS vsnprintf.$ac_objext" if test $ac_cv_func_vsnprintf = yes; then REPLACE_VSNPRINTF=1 fi : fi if test $ac_cv_have_decl_vsnprintf = no; then HAVE_DECL_VSNPRINTF=0 fi GNULIB_VSNPRINTF=1 $as_echo "#define GNULIB_TEST_VSNPRINTF 1" >>confdefs.h if test $gl_cv_have_include_next = yes; then gl_cv_next_wchar_h='<'wchar.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_wchar_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_wchar_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'wchar.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_wchar_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_wchar_h gl_cv_next_wchar_h='"'$gl_header'"' else gl_cv_next_wchar_h='<'wchar.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_wchar_h" >&5 $as_echo "$gl_cv_next_wchar_h" >&6; } fi NEXT_WCHAR_H=$gl_cv_next_wchar_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'wchar.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_wchar_h fi NEXT_AS_FIRST_DIRECTIVE_WCHAR_H=$gl_next_as_first_directive if test $ac_cv_header_wchar_h = yes; then HAVE_WCHAR_H=1 else HAVE_WCHAR_H=0 fi if test $gt_cv_c_wint_t = yes; then HAVE_WINT_T=1 else HAVE_WINT_T=0 fi for gl_func in btowc wctob mbsinit mbrtowc mbrlen mbsrtowcs mbsnrtowcs wcrtomb wcsrtombs wcsnrtombs wcwidth wmemchr wmemcmp wmemcpy wmemmove wmemset wcslen wcsnlen wcscpy wcpcpy wcsncpy wcpncpy wcscat wcsncat wcscmp wcsncmp wcscasecmp wcsncasecmp wcscoll wcsxfrm wcsdup wcschr wcsrchr wcscspn wcsspn wcspbrk wcsstr wcstok wcswidth ; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... 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BSD/OS 4.0.1 has a bug: , and must be included before . */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include # include # include #endif #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done if test $ac_cv_func_mbsinit = yes && test $ac_cv_func_mbrtowc = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc handles incomplete characters" >&5 $as_echo_n "checking whether mbrtowc handles incomplete characters... " >&6; } if ${gl_cv_func_mbrtowc_incomplete_state+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on AIX and OSF/1. aix* | osf*) gl_cv_func_mbrtowc_incomplete_state="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_incomplete_state="guessing yes" ;; esac if test $LOCALE_JA != none; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { const char input[] = "B\217\253\344\217\251\316er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) if (mbsinit (&state)) return 1; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_incomplete_state=yes else gl_cv_func_mbrtowc_incomplete_state=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_incomplete_state" >&5 $as_echo "$gl_cv_func_mbrtowc_incomplete_state" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc works as well as mbtowc" >&5 $as_echo_n "checking whether mbrtowc works as well as mbtowc... " >&6; } if ${gl_cv_func_mbrtowc_sanitycheck+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on Solaris 8. solaris2.8) gl_cv_func_mbrtowc_sanitycheck="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_sanitycheck="guessing yes" ;; esac if test $LOCALE_ZH_CN != none; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { /* This fails on Solaris 8: mbrtowc returns 2, and sets wc to 0x00F0. mbtowc returns 4 (correct) and sets wc to 0x5EDC. */ if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { char input[] = "B\250\271\201\060\211\070er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 6, &state) != 4 && mbtowc (&wc, input + 3, 6) == 4) return 1; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_sanitycheck=yes else gl_cv_func_mbrtowc_sanitycheck=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_sanitycheck" >&5 $as_echo "$gl_cv_func_mbrtowc_sanitycheck" >&6; } REPLACE_MBSTATE_T=0 case "$gl_cv_func_mbrtowc_incomplete_state" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac case "$gl_cv_func_mbrtowc_sanitycheck" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac else REPLACE_MBSTATE_T=1 fi if test $ac_cv_func_wcrtomb = no; then HAVE_WCRTOMB=0 ac_fn_c_check_decl "$LINENO" "wcrtomb" "ac_cv_have_decl_wcrtomb" " /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include " if test "x$ac_cv_have_decl_wcrtomb" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_WCRTOMB $ac_have_decl _ACEOF if test $ac_cv_have_decl_wcrtomb = yes; then REPLACE_WCRTOMB=1 fi else if test $REPLACE_MBSTATE_T = 1; then REPLACE_WCRTOMB=1 else { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether wcrtomb return value is correct" >&5 $as_echo_n "checking whether wcrtomb return value is correct... " >&6; } if ${gl_cv_func_wcrtomb_retval+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on AIX 4, OSF/1 and Solaris. aix4* | osf* | solaris*) gl_cv_func_wcrtomb_retval="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_wcrtomb_retval="guessing yes" ;; esac if test $LOCALE_FR != none || test $LOCALE_FR_UTF8 != none || test $LOCALE_JA != none || test $LOCALE_ZH_CN != none; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { int result = 0; if (setlocale (LC_ALL, "$LOCALE_FR") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 1; } if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 2; } if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 4; } if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 8; } return result; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_wcrtomb_retval=yes else gl_cv_func_wcrtomb_retval=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_wcrtomb_retval" >&5 $as_echo "$gl_cv_func_wcrtomb_retval" >&6; } case "$gl_cv_func_wcrtomb_retval" in *yes) ;; *) REPLACE_WCRTOMB=1 ;; esac fi fi if test $HAVE_WCRTOMB = 0 || test $REPLACE_WCRTOMB = 1; then gl_LIBOBJS="$gl_LIBOBJS wcrtomb.$ac_objext" : fi GNULIB_WCRTOMB=1 $as_echo "#define GNULIB_TEST_WCRTOMB 1" >>confdefs.h if test $ac_cv_func_iswcntrl = yes; then HAVE_ISWCNTRL=1 else HAVE_ISWCNTRL=0 fi if test $gt_cv_c_wint_t = yes; then HAVE_WINT_T=1 else HAVE_WINT_T=0 fi if test $gl_cv_have_include_next = yes; then gl_cv_next_wctype_h='<'wctype.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_wctype_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_wctype_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'wctype.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_wctype_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_wctype_h gl_cv_next_wctype_h='"'$gl_header'"' else gl_cv_next_wctype_h='<'wctype.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_wctype_h" >&5 $as_echo "$gl_cv_next_wctype_h" >&6; } fi NEXT_WCTYPE_H=$gl_cv_next_wctype_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'wctype.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_wctype_h fi NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H=$gl_next_as_first_directive if test $ac_cv_header_wctype_h = yes; then if test $ac_cv_func_iswcntrl = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether iswcntrl works" >&5 $as_echo_n "checking whether iswcntrl works... " >&6; } if ${gl_cv_func_iswcntrl_works+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #if __GNU_LIBRARY__ == 1 Linux libc5 i18n is broken. #endif int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_func_iswcntrl_works="guessing yes" else gl_cv_func_iswcntrl_works="guessing no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #include int main () { return iswprint ('x') == 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_iswcntrl_works=yes else gl_cv_func_iswcntrl_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_iswcntrl_works" >&5 $as_echo "$gl_cv_func_iswcntrl_works" >&6; } fi HAVE_WCTYPE_H=1 else HAVE_WCTYPE_H=0 fi case "$gl_cv_func_iswcntrl_works" in *yes) REPLACE_ISWCNTRL=0 ;; *) REPLACE_ISWCNTRL=1 ;; esac if test $HAVE_ISWCNTRL = 0 || test $REPLACE_ISWCNTRL = 1; then : fi if test $REPLACE_ISWCNTRL = 1; then REPLACE_TOWLOWER=1 else for ac_func in towlower do : ac_fn_c_check_func "$LINENO" "towlower" "ac_cv_func_towlower" if test "x$ac_cv_func_towlower" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_TOWLOWER 1 _ACEOF fi done if test $ac_cv_func_towlower = yes; then REPLACE_TOWLOWER=0 else ac_fn_c_check_decl "$LINENO" "towlower" "ac_cv_have_decl_towlower" "/* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #if HAVE_WCTYPE_H # include #endif " if test "x$ac_cv_have_decl_towlower" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_TOWLOWER $ac_have_decl _ACEOF if test $ac_cv_have_decl_towlower = yes; then REPLACE_TOWLOWER=1 else REPLACE_TOWLOWER=0 fi fi fi if test $HAVE_ISWCNTRL = 0 || test $REPLACE_TOWLOWER = 1; then : fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for wctype_t" >&5 $as_echo_n "checking for wctype_t... " >&6; } if ${gl_cv_type_wctype_t+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #if HAVE_WCTYPE_H # include #endif wctype_t a; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_type_wctype_t=yes else gl_cv_type_wctype_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_type_wctype_t" >&5 $as_echo "$gl_cv_type_wctype_t" >&6; } if test $gl_cv_type_wctype_t = no; then HAVE_WCTYPE_T=0 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for wctrans_t" >&5 $as_echo_n "checking for wctrans_t... " >&6; } if ${gl_cv_type_wctrans_t+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #include wctrans_t a; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_type_wctrans_t=yes else gl_cv_type_wctrans_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_type_wctrans_t" >&5 $as_echo "$gl_cv_type_wctrans_t" >&6; } if test $gl_cv_type_wctrans_t = no; then HAVE_WCTRANS_T=0 fi for gl_func in wctype iswctype wctrans towctrans ; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include # include # include # include #endif #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done for ac_header in stdint.h do : ac_fn_c_check_header_mongrel "$LINENO" "stdint.h" "ac_cv_header_stdint_h" "$ac_includes_default" if test "x$ac_cv_header_stdint_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STDINT_H 1 _ACEOF fi done # End of code from modules gltests_libdeps= gltests_ltlibdeps= gl_source_base='bootstrapped/tests' gltests_WITNESS=IN_`echo "${PACKAGE-$PACKAGE_TARNAME}" | LC_ALL=C tr abcdefghijklmnopqrstuvwxyz ABCDEFGHIJKLMNOPQRSTUVWXYZ | LC_ALL=C sed -e 's/[^A-Z0-9_]/_/g'`_GNULIB_TESTS gl_module_indicator_condition=$gltests_WITNESS { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a traditional french locale" >&5 $as_echo_n "checking for a traditional french locale... " >&6; } if ${gt_cv_locale_fr+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is only one byte long. This excludes the UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 3 || buf[2] != 'v') return 1; #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the native Windows locale name. if (LC_ALL=French_France.1252 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=French_France.1252 else # None found. gt_cv_locale_fr=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.ISO-8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO-8859-1 else # Test for the AIX, OSF/1, FreeBSD, NetBSD, OpenBSD locale name. if (LC_ALL=fr_FR.ISO8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO8859-1 else # Test for the HP-UX locale name. if (LC_ALL=fr_FR.iso88591 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.iso88591 else # Test for the Solaris 7 locale name. if (LC_ALL=fr LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr else # None found. gt_cv_locale_fr=none fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr" >&5 $as_echo "$gt_cv_locale_fr" >&6; } LOCALE_FR=$gt_cv_locale_fr { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a french Unicode locale" >&5 $as_echo_n "checking for a french Unicode locale... " >&6; } if ${gt_cv_locale_fr_utf8+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if !(defined __BEOS__ || defined __HAIKU__) /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr_utf8" >&5 $as_echo "$gt_cv_locale_fr_utf8" >&6; } LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a traditional french locale" >&5 $as_echo_n "checking for a traditional french locale... " >&6; } if ${gt_cv_locale_fr+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is only one byte long. This excludes the UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 3 || buf[2] != 'v') return 1; #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the native Windows locale name. if (LC_ALL=French_France.1252 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=French_France.1252 else # None found. gt_cv_locale_fr=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.ISO-8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO-8859-1 else # Test for the AIX, OSF/1, FreeBSD, NetBSD, OpenBSD locale name. if (LC_ALL=fr_FR.ISO8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO8859-1 else # Test for the HP-UX locale name. if (LC_ALL=fr_FR.iso88591 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.iso88591 else # Test for the Solaris 7 locale name. if (LC_ALL=fr LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr else # None found. gt_cv_locale_fr=none fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr" >&5 $as_echo "$gt_cv_locale_fr" >&6; } LOCALE_FR=$gt_cv_locale_fr { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a turkish Unicode locale" >&5 $as_echo_n "checking for a turkish Unicode locale... " >&6; } if ${gt_cv_locale_tr_utf8+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. But BeOS does not implement the Turkish upper-/lowercase mappings. Therefore, let this program return 1 on BeOS. */ /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the tr_TR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in the abbreviation of the eighth month, the second character (should be U+011F: LATIN SMALL LETTER G WITH BREVE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1992 - 1900; t.tm_mon = 8 - 1; t.tm_mday = 19; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc4 || buf[2] != (char) 0x9f) return 1; /* Check whether the upper-/lowercase mappings are as expected for Turkish. */ if (towupper ('i') != 0x0130 || towlower (0x0130) != 'i' || towupper(0x0131) != 'I' || towlower ('I') != 0x0131) return 1; return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=Turkish_Turkey.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_tr_utf8=Turkish_Turkey.65001 else # None found. gt_cv_locale_tr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. 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" >&6; } if ${ac_cv_c_flexmember+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include struct s { int n; double d[]; }; int main () { int m = getchar (); size_t nbytes = offsetof (struct s, d) + m * sizeof (double); nbytes += sizeof (struct s) - 1; nbytes -= nbytes % sizeof (struct s); struct s *p = malloc (nbytes); p->d[0] = 0.0; return p->d != (double *) NULL; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_c_flexmember=yes else ac_cv_c_flexmember=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_c_flexmember" >&5 $as_echo "$ac_cv_c_flexmember" >&6; } if test $ac_cv_c_flexmember = yes; then $as_echo "#define FLEXIBLE_ARRAY_MEMBER /**/" >>confdefs.h else $as_echo "#define FLEXIBLE_ARRAY_MEMBER 1" >>confdefs.h fi if test $HAVE_MSVC_INVALID_PARAMETER_HANDLER = 1; then REPLACE_FSTAT=1 fi if test $WINDOWS_64_BIT_ST_SIZE = 1; then REPLACE_FSTAT=1 fi if test $REPLACE_FSTAT = 1; then gltests_LIBOBJS="$gltests_LIBOBJS fstat.$ac_objext" : fi if test "$GNULIB_FSTAT" != 1; then if test "$GNULIB_FSTAT" = 0; then GNULIB_FSTAT=$gl_module_indicator_condition else GNULIB_FSTAT="($GNULIB_FSTAT || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_FSTAT 1" >>confdefs.h case $gl_cv_func_getcwd_null,$gl_cv_func_getcwd_posix_signature in *yes,yes) ;; *) REPLACE_GETCWD=1 ;; esac if test $REPLACE_GETCWD = 1; then gltests_LIBOBJS="$gltests_LIBOBJS getcwd-lgpl.$ac_objext" fi if test "$GNULIB_GETCWD" != 1; then if test "$GNULIB_GETCWD" = 0; then GNULIB_GETCWD=$gl_module_indicator_condition else GNULIB_GETCWD="($GNULIB_GETCWD || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_GETCWD 1" >>confdefs.h if test $ac_cv_func_getdtablesize = yes && test $ac_cv_have_decl_getdtablesize = yes; then # Cygwin 1.7.25 automatically increases the RLIMIT_NOFILE soft limit # up to an unchangeable hard limit; all other platforms correctly # require setrlimit before getdtablesize() can report a larger value. { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether getdtablesize works" >&5 $as_echo_n "checking whether getdtablesize works... 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" >&6; } if ${gl_cv_func_gettimeofday_clobber+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : # When cross-compiling: case "$host_os" in # Guess all is fine on glibc systems. *-gnu*) gl_cv_func_gettimeofday_clobber="guessing no" ;; # If we don't know, assume the worst. *) gl_cv_func_gettimeofday_clobber="guessing yes" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #include int main () { time_t t = 0; struct tm *lt; struct tm saved_lt; struct timeval tv; lt = localtime (&t); saved_lt = *lt; gettimeofday (&tv, NULL); return memcmp (lt, &saved_lt, sizeof (struct tm)) != 0; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_gettimeofday_clobber=no else gl_cv_func_gettimeofday_clobber=yes fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_gettimeofday_clobber" >&5 $as_echo "$gl_cv_func_gettimeofday_clobber" >&6; } case "$gl_cv_func_gettimeofday_clobber" in *yes) REPLACE_GETTIMEOFDAY=1 REPLACE_GMTIME=1 REPLACE_LOCALTIME=1 $as_echo "#define GETTIMEOFDAY_CLOBBERS_LOCALTIME 1" >>confdefs.h ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking for gettimeofday with POSIX signature" >&5 $as_echo_n "checking for gettimeofday with POSIX signature... " >&6; } if ${gl_cv_func_gettimeofday_posix_signature+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include struct timeval c; int gettimeofday (struct timeval *restrict, void *restrict); int main () { /* glibc uses struct timezone * rather than the POSIX void * if _GNU_SOURCE is defined. However, since the only portable use of gettimeofday uses NULL as the second parameter, and since the glibc definition is actually more typesafe, it is not worth wrapping this to get a compliant signature. */ int (*f) (struct timeval *restrict, void *restrict) = gettimeofday; int x = f (&c, 0); return !(x | c.tv_sec | c.tv_usec); ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_func_gettimeofday_posix_signature=yes else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int gettimeofday (struct timeval *restrict, struct timezone *restrict); int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_func_gettimeofday_posix_signature=almost else gl_cv_func_gettimeofday_posix_signature=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_gettimeofday_posix_signature" >&5 $as_echo "$gl_cv_func_gettimeofday_posix_signature" >&6; } if test $gl_cv_func_gettimeofday_posix_signature = almost; then gl_gettimeofday_timezone='struct timezone' elif test $gl_cv_func_gettimeofday_posix_signature != yes; then REPLACE_GETTIMEOFDAY=1 fi if test $REPLACE_STRUCT_TIMEVAL = 1; then REPLACE_GETTIMEOFDAY=1 fi fi cat >>confdefs.h <<_ACEOF #define GETTIMEOFDAY_TIMEZONE $gl_gettimeofday_timezone _ACEOF if test $HAVE_GETTIMEOFDAY = 0 || test $REPLACE_GETTIMEOFDAY = 1; then gltests_LIBOBJS="$gltests_LIBOBJS gettimeofday.$ac_objext" for ac_header in sys/timeb.h do : ac_fn_c_check_header_mongrel "$LINENO" "sys/timeb.h" "ac_cv_header_sys_timeb_h" "$ac_includes_default" if test "x$ac_cv_header_sys_timeb_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_SYS_TIMEB_H 1 _ACEOF fi done for ac_func in _ftime do : ac_fn_c_check_func "$LINENO" "_ftime" "ac_cv_func__ftime" if test "x$ac_cv_func__ftime" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE__FTIME 1 _ACEOF fi done fi if test "$GNULIB_GETTIMEOFDAY" != 1; then if test "$GNULIB_GETTIMEOFDAY" = 0; then GNULIB_GETTIMEOFDAY=$gl_module_indicator_condition else GNULIB_GETTIMEOFDAY="($GNULIB_GETTIMEOFDAY || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_GETTIMEOFDAY 1" >>confdefs.h PRIPTR_PREFIX= if test -n "$STDINT_H"; then PRIPTR_PREFIX='"l"' else for glpfx in '' l ll I64; do case $glpfx in '') gltype1='int';; l) gltype1='long int';; ll) gltype1='long long int';; I64) gltype1='__int64';; esac cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include extern intptr_t foo; extern $gltype1 foo; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : PRIPTR_PREFIX='"'$glpfx'"' fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext test -n "$PRIPTR_PREFIX" && break done fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether INT32_MAX < INTMAX_MAX" >&5 $as_echo_n "checking whether INT32_MAX < INTMAX_MAX... 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" >&6; } if ${gt_cv_locale_fr+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is only one byte long. This excludes the UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 3 || buf[2] != 'v') return 1; #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the native Windows locale name. if (LC_ALL=French_France.1252 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=French_France.1252 else # None found. gt_cv_locale_fr=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.ISO-8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO-8859-1 else # Test for the AIX, OSF/1, FreeBSD, NetBSD, OpenBSD locale name. if (LC_ALL=fr_FR.ISO8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO8859-1 else # Test for the HP-UX locale name. if (LC_ALL=fr_FR.iso88591 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.iso88591 else # Test for the Solaris 7 locale name. if (LC_ALL=fr LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr else # None found. gt_cv_locale_fr=none fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr" >&5 $as_echo "$gt_cv_locale_fr" >&6; } LOCALE_FR=$gt_cv_locale_fr { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a french Unicode locale" >&5 $as_echo_n "checking for a french Unicode locale... " >&6; } if ${gt_cv_locale_fr_utf8+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if !(defined __BEOS__ || defined __HAIKU__) /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr_utf8" >&5 $as_echo "$gt_cv_locale_fr_utf8" >&6; } LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a traditional japanese locale" >&5 $as_echo_n "checking for a traditional japanese locale... " >&6; } if ${gt_cv_locale_ja+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { const char *p; /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether MB_CUR_MAX is > 1. This excludes the dysfunctional locales on Cygwin 1.5.x. */ if (MB_CUR_MAX == 1) return 1; /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Note that on native Windows, the Japanese locale is # Japanese_Japan.932, and CP932 is very different from EUC-JP, so we # cannot use it here. gt_cv_locale_ja=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the AIX locale name. if (LC_ALL=ja_JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP else # Test for the locale name with explicit encoding suffix. if (LC_ALL=ja_JP.EUC-JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC-JP else # Test for the HP-UX, OSF/1, NetBSD locale name. if (LC_ALL=ja_JP.eucJP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.eucJP else # Test for the IRIX, FreeBSD locale name. if (LC_ALL=ja_JP.EUC LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC else # Test for the Solaris 7 locale name. if (LC_ALL=ja LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja else # Special test for NetBSD 1.6. if test -f /usr/share/locale/ja_JP.eucJP/LC_CTYPE; then gt_cv_locale_ja=ja_JP.eucJP else # None found. gt_cv_locale_ja=none fi fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_ja" >&5 $as_echo "$gt_cv_locale_ja" >&6; } LOCALE_JA=$gt_cv_locale_ja { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a transitional chinese locale" >&5 $as_echo_n "checking for a transitional chinese locale... " >&6; } if ${gt_cv_locale_zh_CN+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { const char *p; /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; /* Check whether a typical GB18030 multibyte sequence is recognized as a single wide character. This excludes the GB2312 and GBK encodings. */ if (mblen ("\203\062\332\066", 5) != 4) return 1; return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=Chinese_China.54936 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=Chinese_China.54936 else # None found. gt_cv_locale_zh_CN=none fi ;; solaris2.8) # On Solaris 8, the locales zh_CN.GB18030, zh_CN.GBK, zh.GBK are # broken. One witness is the test case in gl_MBRTOWC_SANITYCHECK. # Another witness is that "LC_ALL=zh_CN.GB18030 bash -c true" dumps core. gt_cv_locale_zh_CN=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the locale name without encoding suffix. if (LC_ALL=zh_CN LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN else # Test for the locale name with explicit encoding suffix. if (LC_ALL=zh_CN.GB18030 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN.GB18030 else # None found. gt_cv_locale_zh_CN=none fi fi ;; esac else # If there was a link error, due to mblen(), the system is so old that # it certainly doesn't have a chinese locale. gt_cv_locale_zh_CN=none fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_zh_CN" >&5 $as_echo "$gt_cv_locale_zh_CN" >&6; } LOCALE_ZH_CN=$gt_cv_locale_zh_CN { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a french Unicode locale" >&5 $as_echo_n "checking for a french Unicode locale... " >&6; } if ${gt_cv_locale_fr_utf8+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if !(defined __BEOS__ || defined __HAIKU__) /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr_utf8" >&5 $as_echo "$gt_cv_locale_fr_utf8" >&6; } LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 # Check for mmap(). Don't use AC_FUNC_MMAP, because it checks too much: it # fails on HP-UX 11, because MAP_FIXED mappings do not work. But this is # irrelevant for anonymous mappings. ac_fn_c_check_func "$LINENO" "mmap" "ac_cv_func_mmap" if test "x$ac_cv_func_mmap" = xyes; then : gl_have_mmap=yes else gl_have_mmap=no fi # Try to allow MAP_ANONYMOUS. gl_have_mmap_anonymous=no if test $gl_have_mmap = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking for MAP_ANONYMOUS" >&5 $as_echo_n "checking for MAP_ANONYMOUS... " >&6; } cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #ifdef MAP_ANONYMOUS I cannot identify this map #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "I cannot identify this map" >/dev/null 2>&1; then : gl_have_mmap_anonymous=yes fi rm -f conftest* if test $gl_have_mmap_anonymous != yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #ifdef MAP_ANON I cannot identify this map #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "I cannot identify this map" >/dev/null 2>&1; then : $as_echo "#define MAP_ANONYMOUS MAP_ANON" >>confdefs.h gl_have_mmap_anonymous=yes fi rm -f conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_have_mmap_anonymous" >&5 $as_echo "$gl_have_mmap_anonymous" >&6; } if test $gl_have_mmap_anonymous = yes; then $as_echo "#define HAVE_MAP_ANONYMOUS 1" >>confdefs.h fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a traditional french locale" >&5 $as_echo_n "checking for a traditional french locale... " >&6; } if ${gt_cv_locale_fr+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is only one byte long. This excludes the UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 3 || buf[2] != 'v') return 1; #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the native Windows locale name. if (LC_ALL=French_France.1252 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=French_France.1252 else # None found. gt_cv_locale_fr=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.ISO-8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO-8859-1 else # Test for the AIX, OSF/1, FreeBSD, NetBSD, OpenBSD locale name. if (LC_ALL=fr_FR.ISO8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO8859-1 else # Test for the HP-UX locale name. if (LC_ALL=fr_FR.iso88591 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.iso88591 else # Test for the Solaris 7 locale name. if (LC_ALL=fr LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr else # None found. gt_cv_locale_fr=none fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr" >&5 $as_echo "$gt_cv_locale_fr" >&6; } LOCALE_FR=$gt_cv_locale_fr { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a french Unicode locale" >&5 $as_echo_n "checking for a french Unicode locale... " >&6; } if ${gt_cv_locale_fr_utf8+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if !(defined __BEOS__ || defined __HAIKU__) /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr_utf8" >&5 $as_echo "$gt_cv_locale_fr_utf8" >&6; } LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 case "$host_os" in mingw* | pw*) REPLACE_OPEN=1 ;; *) { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether open recognizes a trailing slash" >&5 $as_echo_n "checking whether open recognizes a trailing slash... " >&6; } if ${gl_cv_func_open_slash+:} false; then : $as_echo_n "(cached) " >&6 else # Assume that if we have lstat, we can also check symlinks. if test $ac_cv_func_lstat = yes; then touch conftest.tmp ln -s conftest.tmp conftest.lnk fi if test "$cross_compiling" = yes; then : case "$host_os" in freebsd* | aix* | hpux* | solaris2.[0-9] | solaris2.[0-9].*) gl_cv_func_open_slash="guessing no" ;; *) gl_cv_func_open_slash="guessing yes" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #if HAVE_UNISTD_H # include #endif int main () { int result = 0; #if HAVE_LSTAT if (open ("conftest.lnk/", O_RDONLY) != -1) result |= 1; #endif if (open ("conftest.sl/", O_CREAT, 0600) >= 0) result |= 2; return result; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_open_slash=yes else gl_cv_func_open_slash=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.sl conftest.tmp conftest.lnk fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_open_slash" >&5 $as_echo "$gl_cv_func_open_slash" >&6; } case "$gl_cv_func_open_slash" in *no) $as_echo "#define OPEN_TRAILING_SLASH_BUG 1" >>confdefs.h REPLACE_OPEN=1 ;; esac ;; esac if test $REPLACE_OPEN = 1; then gltests_LIBOBJS="$gltests_LIBOBJS open.$ac_objext" : fi if test "$GNULIB_OPEN" != 1; then if test "$GNULIB_OPEN" = 0; then GNULIB_OPEN=$gl_module_indicator_condition else GNULIB_OPEN="($GNULIB_OPEN || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_OPEN 1" >>confdefs.h { $as_echo "$as_me:${as_lineno-$LINENO}: checking for putenv compatible with GNU and SVID" >&5 $as_echo_n "checking for putenv compatible with GNU and SVID... " >&6; } if ${gl_cv_func_svid_putenv+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_svid_putenv="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_svid_putenv="guessing no" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ $ac_includes_default int main () { /* Put it in env. */ if (putenv ("CONFTEST_putenv=val")) return 1; /* Try to remove it. */ if (putenv ("CONFTEST_putenv")) return 2; /* Make sure it was deleted. */ if (getenv ("CONFTEST_putenv") != 0) return 3; return 0; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_svid_putenv=yes else gl_cv_func_svid_putenv=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_svid_putenv" >&5 $as_echo "$gl_cv_func_svid_putenv" >&6; } case "$gl_cv_func_svid_putenv" in *yes) ;; *) REPLACE_PUTENV=1 ;; esac if test $REPLACE_PUTENV = 1; then gltests_LIBOBJS="$gltests_LIBOBJS putenv.$ac_objext" ac_fn_c_check_decl "$LINENO" "_putenv" "ac_cv_have_decl__putenv" "$ac_includes_default" if test "x$ac_cv_have_decl__putenv" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL__PUTENV $ac_have_decl _ACEOF fi if test "$GNULIB_PUTENV" != 1; then if test "$GNULIB_PUTENV" = 0; then GNULIB_PUTENV=$gl_module_indicator_condition else GNULIB_PUTENV="($GNULIB_PUTENV || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_PUTENV 1" >>confdefs.h # Check for mmap(). Don't use AC_FUNC_MMAP, because it checks too much: it # fails on HP-UX 11, because MAP_FIXED mappings do not work. But this is # irrelevant for anonymous mappings. ac_fn_c_check_func "$LINENO" "mmap" "ac_cv_func_mmap" if test "x$ac_cv_func_mmap" = xyes; then : gl_have_mmap=yes else gl_have_mmap=no fi # Try to allow MAP_ANONYMOUS. gl_have_mmap_anonymous=no if test $gl_have_mmap = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking for MAP_ANONYMOUS" >&5 $as_echo_n "checking for MAP_ANONYMOUS... " >&6; } cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #ifdef MAP_ANONYMOUS I cannot identify this map #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "I cannot identify this map" >/dev/null 2>&1; then : gl_have_mmap_anonymous=yes fi rm -f conftest* if test $gl_have_mmap_anonymous != yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #ifdef MAP_ANON I cannot identify this map #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "I cannot identify this map" >/dev/null 2>&1; then : $as_echo "#define MAP_ANONYMOUS MAP_ANON" >>confdefs.h gl_have_mmap_anonymous=yes fi rm -f conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_have_mmap_anonymous" >&5 $as_echo "$gl_have_mmap_anonymous" >&6; } if test $gl_have_mmap_anonymous = yes; then $as_echo "#define HAVE_MAP_ANONYMOUS 1" >>confdefs.h fi fi if test $ac_cv_func_setenv = no; then HAVE_SETENV=0 else { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether setenv validates arguments" >&5 $as_echo_n "checking whether setenv validates arguments... " >&6; } if ${gl_cv_func_setenv_works+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_setenv_works="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_setenv_works="guessing no" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include int main () { int result = 0; { if (setenv ("", "", 0) != -1) result |= 1; else if (errno != EINVAL) result |= 2; } { if (setenv ("a", "=", 1) != 0) result |= 4; else if (strcmp (getenv ("a"), "=") != 0) result |= 8; } return result; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_setenv_works=yes else gl_cv_func_setenv_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_setenv_works" >&5 $as_echo "$gl_cv_func_setenv_works" >&6; } case "$gl_cv_func_setenv_works" in *yes) ;; *) REPLACE_SETENV=1 ;; esac fi if test $HAVE_SETENV = 0 || test $REPLACE_SETENV = 1; then gltests_LIBOBJS="$gltests_LIBOBJS setenv.$ac_objext" fi if test "$GNULIB_SETENV" != 1; then if test "$GNULIB_SETENV" = 0; then GNULIB_SETENV=$gl_module_indicator_condition else GNULIB_SETENV="($GNULIB_SETENV || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_SETENV 1" >>confdefs.h case "$host_os" in mingw*) REPLACE_SETLOCALE=1 ;; cygwin*) case `uname -r` in 1.5.*) REPLACE_SETLOCALE=1 ;; esac ;; esac if test $REPLACE_SETLOCALE = 1; then gltests_LIBOBJS="$gltests_LIBOBJS setlocale.$ac_objext" : fi if test "$GNULIB_SETLOCALE" != 1; then if test "$GNULIB_SETLOCALE" = 0; then GNULIB_SETLOCALE=$gl_module_indicator_condition else GNULIB_SETLOCALE="($GNULIB_SETLOCALE || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_SETLOCALE 1" >>confdefs.h { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a traditional french locale" >&5 $as_echo_n "checking for a traditional french locale... " >&6; } if ${gt_cv_locale_fr+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is only one byte long. This excludes the UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 3 || buf[2] != 'v') return 1; #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the native Windows locale name. if (LC_ALL=French_France.1252 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=French_France.1252 else # None found. gt_cv_locale_fr=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.ISO-8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO-8859-1 else # Test for the AIX, OSF/1, FreeBSD, NetBSD, OpenBSD locale name. if (LC_ALL=fr_FR.ISO8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO8859-1 else # Test for the HP-UX locale name. if (LC_ALL=fr_FR.iso88591 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.iso88591 else # Test for the Solaris 7 locale name. if (LC_ALL=fr LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr else # None found. gt_cv_locale_fr=none fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr" >&5 $as_echo "$gt_cv_locale_fr" >&6; } LOCALE_FR=$gt_cv_locale_fr { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a french Unicode locale" >&5 $as_echo_n "checking for a french Unicode locale... " >&6; } if ${gt_cv_locale_fr_utf8+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if !(defined __BEOS__ || defined __HAIKU__) /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr_utf8" >&5 $as_echo "$gt_cv_locale_fr_utf8" >&6; } LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a traditional japanese locale" >&5 $as_echo_n "checking for a traditional japanese locale... " >&6; } if ${gt_cv_locale_ja+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { const char *p; /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether MB_CUR_MAX is > 1. This excludes the dysfunctional locales on Cygwin 1.5.x. */ if (MB_CUR_MAX == 1) return 1; /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Note that on native Windows, the Japanese locale is # Japanese_Japan.932, and CP932 is very different from EUC-JP, so we # cannot use it here. gt_cv_locale_ja=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the AIX locale name. if (LC_ALL=ja_JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP else # Test for the locale name with explicit encoding suffix. if (LC_ALL=ja_JP.EUC-JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC-JP else # Test for the HP-UX, OSF/1, NetBSD locale name. if (LC_ALL=ja_JP.eucJP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.eucJP else # Test for the IRIX, FreeBSD locale name. if (LC_ALL=ja_JP.EUC LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC else # Test for the Solaris 7 locale name. if (LC_ALL=ja LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja else # Special test for NetBSD 1.6. if test -f /usr/share/locale/ja_JP.eucJP/LC_CTYPE; then gt_cv_locale_ja=ja_JP.eucJP else # None found. gt_cv_locale_ja=none fi fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_ja" >&5 $as_echo "$gt_cv_locale_ja" >&6; } LOCALE_JA=$gt_cv_locale_ja { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a transitional chinese locale" >&5 $as_echo_n "checking for a transitional chinese locale... " >&6; } if ${gt_cv_locale_zh_CN+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { const char *p; /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; /* Check whether a typical GB18030 multibyte sequence is recognized as a single wide character. This excludes the GB2312 and GBK encodings. */ if (mblen ("\203\062\332\066", 5) != 4) return 1; return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=Chinese_China.54936 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=Chinese_China.54936 else # None found. gt_cv_locale_zh_CN=none fi ;; solaris2.8) # On Solaris 8, the locales zh_CN.GB18030, zh_CN.GBK, zh.GBK are # broken. One witness is the test case in gl_MBRTOWC_SANITYCHECK. # Another witness is that "LC_ALL=zh_CN.GB18030 bash -c true" dumps core. gt_cv_locale_zh_CN=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. 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" >&6; } if ${gl_cv_func_symlink_works+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_symlink_works="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_symlink_works="guessing no" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { int result = 0; if (!symlink ("a", "conftest.link/")) result |= 1; if (symlink ("conftest.f", "conftest.lnk2")) result |= 2; else if (!symlink ("a", "conftest.lnk2/")) result |= 4; return result; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_symlink_works=yes else gl_cv_func_symlink_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.f conftest.link conftest.lnk2 fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_symlink_works" >&5 $as_echo "$gl_cv_func_symlink_works" >&6; } case "$gl_cv_func_symlink_works" in *yes) ;; *) REPLACE_SYMLINK=1 ;; esac fi if test $HAVE_SYMLINK = 0 || test $REPLACE_SYMLINK = 1; then gltests_LIBOBJS="$gltests_LIBOBJS symlink.$ac_objext" fi if test "$GNULIB_SYMLINK" != 1; then if test "$GNULIB_SYMLINK" = 0; then GNULIB_SYMLINK=$gl_module_indicator_condition else GNULIB_SYMLINK="($GNULIB_SYMLINK || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_SYMLINK 1" >>confdefs.h if test $gl_cv_have_include_next = yes; then gl_cv_next_sys_stat_h='<'sys/stat.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... 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" >&6; } if ${gt_cv_func_unsetenv_ret+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #undef _BSD #define _BSD 1 /* unhide unsetenv declaration in OSF/1 5.1 */ #include extern #ifdef __cplusplus "C" #endif int unsetenv (const char *name); int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gt_cv_func_unsetenv_ret='int' else gt_cv_func_unsetenv_ret='void' fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_func_unsetenv_ret" >&5 $as_echo "$gt_cv_func_unsetenv_ret" >&6; } if test $gt_cv_func_unsetenv_ret = 'void'; then $as_echo "#define VOID_UNSETENV 1" >>confdefs.h REPLACE_UNSETENV=1 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether unsetenv obeys POSIX" >&5 $as_echo_n "checking whether unsetenv obeys POSIX... 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Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is only one byte long. This excludes the UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 3 || buf[2] != 'v') return 1; #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the native Windows locale name. if (LC_ALL=French_France.1252 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=French_France.1252 else # None found. gt_cv_locale_fr=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. 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Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr_utf8" >&5 $as_echo "$gt_cv_locale_fr_utf8" >&6; } LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a traditional japanese locale" >&5 $as_echo_n "checking for a traditional japanese locale... " >&6; } if ${gt_cv_locale_ja+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { const char *p; /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether MB_CUR_MAX is > 1. This excludes the dysfunctional locales on Cygwin 1.5.x. */ if (MB_CUR_MAX == 1) return 1; /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Note that on native Windows, the Japanese locale is # Japanese_Japan.932, and CP932 is very different from EUC-JP, so we # cannot use it here. gt_cv_locale_ja=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the AIX locale name. if (LC_ALL=ja_JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP else # Test for the locale name with explicit encoding suffix. if (LC_ALL=ja_JP.EUC-JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC-JP else # Test for the HP-UX, OSF/1, NetBSD locale name. if (LC_ALL=ja_JP.eucJP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.eucJP else # Test for the IRIX, FreeBSD locale name. if (LC_ALL=ja_JP.EUC LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC else # Test for the Solaris 7 locale name. if (LC_ALL=ja LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja else # Special test for NetBSD 1.6. if test -f /usr/share/locale/ja_JP.eucJP/LC_CTYPE; then gt_cv_locale_ja=ja_JP.eucJP else # None found. gt_cv_locale_ja=none fi fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_ja" >&5 $as_echo "$gt_cv_locale_ja" >&6; } LOCALE_JA=$gt_cv_locale_ja { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a transitional chinese locale" >&5 $as_echo_n "checking for a transitional chinese locale... " >&6; } if ${gt_cv_locale_zh_CN+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { const char *p; /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; /* Check whether a typical GB18030 multibyte sequence is recognized as a single wide character. This excludes the GB2312 and GBK encodings. */ if (mblen ("\203\062\332\066", 5) != 4) return 1; return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=Chinese_China.54936 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=Chinese_China.54936 else # None found. gt_cv_locale_zh_CN=none fi ;; solaris2.8) # On Solaris 8, the locales zh_CN.GB18030, zh_CN.GBK, zh.GBK are # broken. One witness is the test case in gl_MBRTOWC_SANITYCHECK. # Another witness is that "LC_ALL=zh_CN.GB18030 bash -c true" dumps core. gt_cv_locale_zh_CN=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the locale name without encoding suffix. if (LC_ALL=zh_CN LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN else # Test for the locale name with explicit encoding suffix. if (LC_ALL=zh_CN.GB18030 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN.GB18030 else # None found. gt_cv_locale_zh_CN=none fi fi ;; esac else # If there was a link error, due to mblen(), the system is so old that # it certainly doesn't have a chinese locale. gt_cv_locale_zh_CN=none fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_zh_CN" >&5 $as_echo "$gt_cv_locale_zh_CN" >&6; } LOCALE_ZH_CN=$gt_cv_locale_zh_CN if test $ac_cv_func_wctob = no; then HAVE_WCTOB=0 HAVE_DECL_WCTOB=0 else HAVE_WCTOB=1 { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether wctob works" >&5 $as_echo_n "checking whether wctob works... " >&6; } if ${gl_cv_func_wctob_works+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on Solaris <= 9 and Cygwin. solaris2.[1-9] | solaris2.[1-9].* | cygwin*) gl_cv_func_wctob_works="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_wctob_works="guessing yes" ;; esac case "$host_os" in cygwin*) if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include register long global __asm__ ("%ebx"); int main () { setlocale (LC_ALL, "en_US.UTF-8"); global = 0x12345678; if (wctob (0x00FC) != -1) return 1; if (global != 0x12345678) return 2; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : : else gl_cv_func_wctob_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi ;; esac if test "$gl_cv_func_wctob_works" != no && test $LOCALE_FR != none; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_FR") != NULL) { wchar_t wc; if (mbtowc (&wc, "\374", 1) == 1) if (wctob (wc) != (unsigned char) '\374') return 1; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_wctob_works=yes else gl_cv_func_wctob_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_wctob_works" >&5 $as_echo "$gl_cv_func_wctob_works" >&6; } case "$gl_cv_func_wctob_works" in *yes) ;; *) REPLACE_WCTOB=1 ;; esac if test $REPLACE_WCTOB = 0; then ac_fn_c_check_decl "$LINENO" "wctob" "ac_cv_have_decl_wctob" " /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include " if test "x$ac_cv_have_decl_wctob" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_WCTOB $ac_have_decl _ACEOF if test $ac_cv_have_decl_wctob != yes; then HAVE_DECL_WCTOB=0 fi fi fi if test $HAVE_WCTOB = 0 || test $REPLACE_WCTOB = 1; then gltests_LIBOBJS="$gltests_LIBOBJS wctob.$ac_objext" : fi if test "$GNULIB_WCTOB" != 1; then if test "$GNULIB_WCTOB" = 0; then GNULIB_WCTOB=$gl_module_indicator_condition else GNULIB_WCTOB="($GNULIB_WCTOB || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_WCTOB 1" >>confdefs.h if false; then REPLACE_WCTOMB=1 fi if test $REPLACE_WCTOMB = 1; then gltests_LIBOBJS="$gltests_LIBOBJS wctomb.$ac_objext" : fi if test "$GNULIB_WCTOMB" != 1; then if test "$GNULIB_WCTOMB" = 0; then GNULIB_WCTOMB=$gl_module_indicator_condition else GNULIB_WCTOMB="($GNULIB_WCTOMB || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_WCTOMB 1" >>confdefs.h YIELD_LIB= if test $gl_threads_api = posix; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking for sched_yield in -lrt" >&5 $as_echo_n "checking for sched_yield in -lrt... " >&6; } if ${ac_cv_lib_rt_sched_yield+:} false; then : $as_echo_n "(cached) " >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lrt $LIBS" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. 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Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char jpeg_stdio_dest (); int main () { return jpeg_stdio_dest (); ; return 0; } _ACEOF for ac_lib in '' jpeg; do if test -z "$ac_lib"; then ac_res="none required" else ac_res=-l$ac_lib LIBS="-l$ac_lib $ac_func_search_save_LIBS" fi if ac_fn_c_try_link "$LINENO"; then : ac_cv_search_jpeg_stdio_dest=$ac_res fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext if ${ac_cv_search_jpeg_stdio_dest+:} false; then : break fi done if ${ac_cv_search_jpeg_stdio_dest+:} false; then : else ac_cv_search_jpeg_stdio_dest=no fi rm conftest.$ac_ext LIBS=$ac_func_search_save_LIBS fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_search_jpeg_stdio_dest" >&5 $as_echo "$ac_cv_search_jpeg_stdio_dest" >&6; } ac_res=$ac_cv_search_jpeg_stdio_dest if test "$ac_res" != no; then : test "$ac_res" = "none required" || LIBS="$ac_res $LIBS" has_libjpeg=yes else has_libjpeg=no fi if test "x$has_libjpeg" = "xyes"; then : $as_echo "#define HAVE_LIBJPEG /**/" >>confdefs.h else anywarnings=yes fi if test "x$has_libjpeg" = "xyes"; then COND_HASLIBJPEG_TRUE= COND_HASLIBJPEG_FALSE='#' else COND_HASLIBJPEG_TRUE='#' COND_HASLIBJPEG_FALSE= fi # Check libgit2: { $as_echo "$as_me:${as_lineno-$LINENO}: checking for library containing git_libgit2_init" >&5 $as_echo_n "checking for library containing git_libgit2_init... " >&6; } if ${ac_cv_search_git_libgit2_init+:} false; then : $as_echo_n "(cached) " >&6 else ac_func_search_save_LIBS=$LIBS cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char git_libgit2_init (); int main () { return git_libgit2_init (); ; return 0; } _ACEOF for ac_lib in '' git2; do if test -z "$ac_lib"; then ac_res="none required" else ac_res=-l$ac_lib LIBS="-l$ac_lib $ac_func_search_save_LIBS" fi if ac_fn_c_try_link "$LINENO"; then : ac_cv_search_git_libgit2_init=$ac_res fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext if ${ac_cv_search_git_libgit2_init+:} false; then : break fi done if ${ac_cv_search_git_libgit2_init+:} false; then : else ac_cv_search_git_libgit2_init=no fi rm conftest.$ac_ext LIBS=$ac_func_search_save_LIBS fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_search_git_libgit2_init" >&5 $as_echo "$ac_cv_search_git_libgit2_init" >&6; } ac_res=$ac_cv_search_git_libgit2_init if test "$ac_res" != no; then : test "$ac_res" = "none required" || LIBS="$ac_res $LIBS" has_libgit2=1 else has_libgit2=0 fi cat >>confdefs.h <<_ACEOF #define GAL_GNUASTRO_HAVE_LIBGIT2 $has_libgit2 _ACEOF if test "x$has_libgit2" = "x1"; then : else anywarnings=yes fi HAVE_LIBGIT2=$has_libgit2 # Check Ghostscript: "-dPDFFitPage" option to Ghostscript, used by # ConvertType to convert from EPS to PDF, has been introduced in # Ghostscript 9.10. Make sure we have at least that version. # # Below, only when Ghostscript exists, we check its version and only if its # version is larger than 9.10, does Gnuastro finally assume the existence # of Ghostscript. AX_COMPARE_VERSION comes from the GNU Autoconf Archive's # ax_compare_version.m4. # Extract the first word of "gs", so it can be a program name with args. set dummy gs; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_has_ghostscript+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$has_ghostscript"; then ac_cv_prog_has_ghostscript="$has_ghostscript" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_has_ghostscript="yes" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS test -z "$ac_cv_prog_has_ghostscript" && ac_cv_prog_has_ghostscript="no" fi fi has_ghostscript=$ac_cv_prog_has_ghostscript if test -n "$has_ghostscript"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $has_ghostscript" >&5 $as_echo "$has_ghostscript" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$has_ghostscript" = "xyes"; then : { $as_echo "$as_me:${as_lineno-$LINENO}: checking Ghostscript version" >&5 $as_echo_n "checking Ghostscript version... " >&6; } gsversion=$(gs --version) # Used to indicate true or false condition ax_compare_version=false # Convert the two version strings to be compared into a format that # allows a simple string comparison. The end result is that a version # string of the form 1.12.5-r617 will be converted to the form # 0001001200050617. 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See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Sources to be created before everything else ## ============================================ ## ## These target(s) will be created before anything else when running ## `make', `make check', or `make install', see the "Built sources" section ## of the AUTOMAKE manual and the git-version-gen script comments for more ## information. Note that AUTHORS depends on `$(top_srcdir)/.version', and ## `$(top_srcdir)/.version' depends on $(top_srcdir)/configure'. So any ## time the version is updated, both of these will be re-built. But during ## usual utility and library development, `$(top_srcdir)/configure' is not ## commonly updated, so this will not slow down the process. BUILT_SOURCES = $(top_srcdir)/AUTHORS ## Directories to check: ## ===================== ## ## Gnulib is intentionally compiled and tested prior to the gnuastro ## progams. With this configuration, the user can confirm if the ## problem is internal to gnulib or still persists after all the ## Gnulib tests have been done. if COND_ARITHMETIC MAYBE_ARITHMETIC = bin/arithmetic endif if COND_CONVERTT MAYBE_CONVERTT = bin/convertt endif if COND_CONVOLVE MAYBE_CONVOLVE = bin/convolve endif if COND_COSMICCAL MAYBE_COSMICCAL = bin/cosmiccal endif if COND_HEADER MAYBE_HEADER = bin/header endif if COND_IMGCROP MAYBE_IMGCROP = bin/imgcrop endif if COND_IMGSTAT MAYBE_IMGSTAT = bin/imgstat endif if COND_IMGWARP MAYBE_IMGWARP = bin/imgwarp endif if COND_MKCATALOG MAYBE_MKCATALOG = bin/mkcatalog endif if COND_MKNOISE MAYBE_MKNOISE = bin/mknoise endif if COND_MKPROF MAYBE_MKPROF = bin/mkprof endif if COND_NOISECHISEL MAYBE_NOISECHISEL = bin/noisechisel endif if COND_SUBTRACTSKY MAYBE_SUBTRACTSKY = bin/subtractsky endif if COND_TABLE MAYBE_TABLE = bin/table endif #if COND_TEMPLATE # MAYBE_TEMPLATE = bin/TEMPLATE #endif if COND_GNULIBCHECK MAYBE_GNULIBCHECK = bootstrapped/tests endif ## Subdirectories to build ## ======================= ## ## Note that by default `COND_TEMPLATE' is not set in configure, it is ## commented, and exists only as a template for you to copy and paste to ## name your new utility. The same rule is applied here (in the `if' ## conditions above). When `MAYBE_TEMPLATE' is not defined, then Make will ## see it as a blank string and igonore it, so there is no problem with ## having an uncommented `MAYBE_TEMPLATE' as a value in `SUBDIRS'. 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Make will ## set MAKECMDGOALS to blank if there are no arguments, however, the way ## Automake works, its value is set to "all-am". all-local: @if [ x$(MAKECMDGOALS) = x"all-am" ] && [ x$(GUIDEMESSAGE) = xyes ]; then \ echo; \ echo "==================================================================="; \ echo "==================================================================="; \ echo "Gnuastro $(VERSION), was successfully built."; \ echo "Please check the build on your system by running:"; \ echo; \ echo " make check"; \ echo; \ echo "(Check faster on N threads with 'make check -jN'.)"; \ echo "(The following \"Leaving directory\" notices can be ignored.)"; \ echo "==================================================================="; \ echo "==================================================================="; \ echo; \ fi ## We cannot do the writing persmission test at configure time. 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This note is mostly for beginners and it is not written to convey ## that this is the ONLY solution. check-local: @if [ x$(GUIDEMESSAGE) = xyes ]; then \ echo; \ echo "==================================================================="; \ echo "==================================================================="; \ echo "Your build of Gnuastro $(VERSION) didn't fail on any tests."; \ echo "To install Gnuastro, please run the commands below:"; \ echo; \ if [ ! -w $(prefix) ] ; then \ echo "(NOTE: As the user $$USER, you don't have writing permissions"; \ echo "in \"$(prefix)\". To install Gnuastro there, you must get "; \ echo "privileges first, as described below. If you can't, configure "; \ echo "Gnuastro again, for example: \"./configure --prefix ~/.local\".)"; \ echo; \ echo " sudo make install"; \ echo "or"; \ echo " su"; \ fi; \ echo " make install"; \ if [ ! -w $(prefix) ] ; then \ echo " exit"; \ fi; \ echo; \ echo "(The following \"Leaving directory\" notices can be ignored.)"; \ echo "==================================================================="; \ echo "==================================================================="; \ echo; \ fi ## Note that the `\' characters in the GNU head here are not printed on the ## command line. So we have to consider them. The ASCII GNU head is taken ## from: https://www.gnu.org/graphics/gnu-ascii.html install-exec-local: @if [ x$(GUIDEMESSAGE) = xyes ]; then \ echo; \ echo "==================================================================="; \ echo "==================================================================="; \ echo " , , "; \ echo " / \ "; \ echo " ((__-^^-,-^^-__)) Congratulations!"; \ echo " \`-_---' \`---_-' GNU Astronomy Utilities (Gnuastro),"; \ echo " \`--|o\` 'o|--' Version $(VERSION)"; \ echo " \ \` / "; \ echo " ): :( Successfully installed on this system."; \ echo " :o_o: "; \ echo " \"-\" "; \ echo; \ echo "More information Command to run "; \ echo "---------------- -------------- "; \ echo "Complete official Gnuastro book: ' info gnuastro '"; \ echo "Entertaining tutorials: ' info gnuastro Tutorials '"; \ echo "Dedicated help mailing list: ' info help-gnuastro '"; \ echo "Instructions for reporting bugs: ' info bug-gnuastro '"; \ echo "Effectively use Info: ' info info '"; \ echo; \ echo; \ echo "Environment variables to check: "; \ echo " - '$(prefix)/bin' in PATH."; \ echo "(for an intro, run 'info gnuastro \"Installation directory\"')"; \ echo; \ echo; \ echo "To stay up to date with future releases, please subscribe to: "; \ echo " https://lists.gnu.org/mailman/listinfo/info-gnuastro"; \ echo; \ echo; \ echo "(The following lines can be ignored.)"; \ echo "==================================================================="; \ echo "==================================================================="; \ echo; \ fi ## $(top_srcdir)/.version ## ====================== ## ## This file is created from the $(VERSION) variable which was defined by ## the `git-version-gen' script (located at address below), which is run ## when the `$(top_srcdir)/configure' script is being built by Autoconf. ## ## $(top_srcdir)/bootstrapped/build-aux/git-version-gen ## ## Note that contrary to what is proposed by `git-version-gen', here the ## creation of `$(top_srcdir)/.version' depends on the ## `$(top_srcdir)/configure' script. Therefore, anytime a the VERSION ## variable is updated there, `$(top_srcdir)/.version' is also ## updated. During development, of the main functionality of Gnuastro ## (utilities and libraries), the `$(top_srcdir/configure' script is rarely ## updated, so `$(top_srcdir)/.version' will not be rebuilt and thus it ## won't harm the speed of tests during development. $(top_srcdir)/.version: $(top_srcdir)/configure echo $(VERSION) > $@-t && mv $@-t $@ ## $(top_srcdir)/AUTHORS ## ===================== ## ## This file is generated automatically from the version controlled ## history. Note the following: ## ## - `$(top_srcdir)/AUTHORS' is defined as a BUILT_SOURCES variable, so ## it is the first thing that is built (even in multi-threaded runs). ## ## - `$(top_srcdir)/AUTHORS' is updated only when ## `$(top_srcdir)/.version' is updated. `$(top_srcdir)/.version' its ## self is only updated when `$(top_srcdir)/configure' is updated. But ## generally, the `$(top_srcdir)/configure' script is not updated ## regularly during development and outside of version control. ## ## - The `$(top_srcdir)/genauthors' script will not do anything ## (make/update the `$(top_srcdir)AUTHORS' file) when there is no git ## repository. `$(top_srcdir)/AUTHORS' is only necessary when building ## a tarball distribution. $(top_srcdir)/AUTHORS: $(top_srcdir)/.version $(top_srcdir)/genauthors $(top_srcdir) ## Run when building a distribution ## ================================ ## ## These targets will be created when building a (tarball) ## distribution. Note that AUTHORS depends on `.version'. dist-hook: $(top_srcdir)/AUTHORS echo $(VERSION) > $(distdir)/.tarball-version gnuastro-0.2.33-8a3b/bootstrapped/0000755000175000017500000000000013004464725013710 500000000000000gnuastro-0.2.33-8a3b/bootstrapped/doc/0000755000175000017500000000000013004464725014455 500000000000000gnuastro-0.2.33-8a3b/bootstrapped/doc/fdl.texi0000644000175000017500000005561013004436754016045 00000000000000@c The GNU Free Documentation License. @center Version 1.3, 3 November 2008 @c This file is intended to be included within another document, @c hence no sectioning command or @node. @display Copyright @copyright{} 2000, 2001, 2002, 2007, 2008 Free Software Foundation, Inc. @uref{http://fsf.org/} Everyone is permitted to copy and distribute verbatim copies of this license document, but changing it is not allowed. @end display @enumerate 0 @item PREAMBLE The purpose of this License is to make a manual, textbook, or other functional and useful document @dfn{free} in the sense of freedom: to assure everyone the effective freedom to copy and redistribute it, with or without modifying it, either commercially or noncommercially. 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If the Cover Text requirement of section 3 is applicable to these copies of the Document, then if the Document is less than one half of the entire aggregate, the Document's Cover Texts may be placed on covers that bracket the Document within the aggregate, or the electronic equivalent of covers if the Document is in electronic form. Otherwise they must appear on printed covers that bracket the whole aggregate. @item TRANSLATION Translation is considered a kind of modification, so you may distribute translations of the Document under the terms of section 4. Replacing Invariant Sections with translations requires special permission from their copyright holders, but you may include translations of some or all Invariant Sections in addition to the original versions of these Invariant Sections. You may include a translation of this License, and all the license notices in the Document, and any Warranty Disclaimers, provided that you also include the original English version of this License and the original versions of those notices and disclaimers. In case of a disagreement between the translation and the original version of this License or a notice or disclaimer, the original version will prevail. If a section in the Document is Entitled ``Acknowledgements'', ``Dedications'', or ``History'', the requirement (section 4) to Preserve its Title (section 1) will typically require changing the actual title. @item TERMINATION You may not copy, modify, sublicense, or distribute the Document except as expressly provided under this License. Any attempt otherwise to copy, modify, sublicense, or distribute it is void, and will automatically terminate your rights under this License. However, if you cease all violation of this License, then your license from a particular copyright holder is reinstated (a) provisionally, unless and until the copyright holder explicitly and finally terminates your license, and (b) permanently, if the copyright holder fails to notify you of the violation by some reasonable means prior to 60 days after the cessation. Moreover, your license from a particular copyright holder is reinstated permanently if the copyright holder notifies you of the violation by some reasonable means, this is the first time you have received notice of violation of this License (for any work) from that copyright holder, and you cure the violation prior to 30 days after your receipt of the notice. Termination of your rights under this section does not terminate the licenses of parties who have received copies or rights from you under this License. If your rights have been terminated and not permanently reinstated, receipt of a copy of some or all of the same material does not give you any rights to use it. @item FUTURE REVISIONS OF THIS LICENSE The Free Software Foundation may publish new, revised versions of the GNU Free Documentation License from time to time. Such new versions will be similar in spirit to the present version, but may differ in detail to address new problems or concerns. See @uref{http://www.gnu.org/copyleft/}. Each version of the License is given a distinguishing version number. If the Document specifies that a particular numbered version of this License ``or any later version'' applies to it, you have the option of following the terms and conditions either of that specified version or of any later version that has been published (not as a draft) by the Free Software Foundation. If the Document does not specify a version number of this License, you may choose any version ever published (not as a draft) by the Free Software Foundation. If the Document specifies that a proxy can decide which future versions of this License can be used, that proxy's public statement of acceptance of a version permanently authorizes you to choose that version for the Document. @item RELICENSING ``Massive Multiauthor Collaboration Site'' (or ``MMC Site'') means any World Wide Web server that publishes copyrightable works and also provides prominent facilities for anybody to edit those works. A public wiki that anybody can edit is an example of such a server. A ``Massive Multiauthor Collaboration'' (or ``MMC'') contained in the site means any set of copyrightable works thus published on the MMC site. ``CC-BY-SA'' means the Creative Commons Attribution-Share Alike 3.0 license published by Creative Commons Corporation, a not-for-profit corporation with a principal place of business in San Francisco, California, as well as future copyleft versions of that license published by that same organization. ``Incorporate'' means to publish or republish a Document, in whole or in part, as part of another Document. An MMC is ``eligible for relicensing'' if it is licensed under this License, and if all works that were first published under this License somewhere other than this MMC, and subsequently incorporated in whole or in part into the MMC, (1) had no cover texts or invariant sections, and (2) were thus incorporated prior to November 1, 2008. The operator of an MMC Site may republish an MMC contained in the site under CC-BY-SA on the same site at any time before August 1, 2009, provided the MMC is eligible for relicensing. @end enumerate @page @heading ADDENDUM: How to use this License for your documents To use this License in a document you have written, include a copy of the License in the document and put the following copyright and license notices just after the title page: @smallexample @group Copyright (C) @var{year} @var{your name}. Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled ``GNU Free Documentation License''. @end group @end smallexample If you have Invariant Sections, Front-Cover Texts and Back-Cover Texts, replace the ``with@dots{}Texts.''@: line with this: @smallexample @group with the Invariant Sections being @var{list their titles}, with the Front-Cover Texts being @var{list}, and with the Back-Cover Texts being @var{list}. @end group @end smallexample If you have Invariant Sections without Cover Texts, or some other combination of the three, merge those two alternatives to suit the situation. If your document contains nontrivial examples of program code, we recommend releasing these examples in parallel under your choice of free software license, such as the GNU General Public License, to permit their use in free software. @c Local Variables: @c ispell-local-pdict: "ispell-dict" @c End: gnuastro-0.2.33-8a3b/bootstrapped/tests/0000755000175000017500000000000013004464724015051 500000000000000gnuastro-0.2.33-8a3b/bootstrapped/tests/wctomb-impl.h0000644000175000017500000000211213004436756017374 00000000000000/* Convert wide character to multibyte character. Copyright (C) 2011-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2011. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ int wctomb (char *s, wchar_t wc) { if (s == NULL) return 0; else { mbstate_t state; size_t result; memset (&state, 0, sizeof (mbstate_t)); result = wcrtomb (s, wc, &state); if (result == (size_t)-1) return -1; return result; } } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-wcrtomb-w32-5.sh0000755000175000017500000000012013004436756020532 00000000000000#!/bin/sh # Test a CP936 locale. ./test-wcrtomb-w32${EXEEXT} Chinese_China 936 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-wcrtomb-w32-4.sh0000755000175000017500000000012113004436756020532 00000000000000#!/bin/sh # Test a CP950 locale. ./test-wcrtomb-w32${EXEEXT} Chinese_Taiwan 950 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-wcrtomb-w32-3.sh0000755000175000017500000000012113004436756020531 00000000000000#!/bin/sh # Test a CP932 locale. ./test-wcrtomb-w32${EXEEXT} Japanese_Japan 932 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-wcrtomb-w32-2.sh0000755000175000017500000000013213004436756020532 00000000000000#!/bin/sh # Test a CP1256 locale. ./test-wcrtomb-w32${EXEEXT} "Arabic_Saudi Arabia" 1256 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-wcrtomb-w32-1.sh0000755000175000017500000000012213004436756020530 00000000000000#!/bin/sh # Test a CP1252 locale. ./test-wcrtomb-w32${EXEEXT} French_France 1252 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-wcrtomb.sh0000755000175000017500000000136113004436756017767 00000000000000#!/bin/sh # Test in an ISO-8859-1 or ISO-8859-15 locale. : ${LOCALE_FR=fr_FR} if test $LOCALE_FR != none; then LC_ALL=$LOCALE_FR \ ./test-wcrtomb${EXEEXT} 1 \ || exit 1 fi # Test whether a specific UTF-8 locale is installed. : ${LOCALE_FR_UTF8=fr_FR.UTF-8} if test $LOCALE_FR_UTF8 != none; then LC_ALL=$LOCALE_FR_UTF8 \ ./test-wcrtomb${EXEEXT} 2 \ || exit 1 fi # Test whether a specific EUC-JP locale is installed. : ${LOCALE_JA=ja_JP} if test $LOCALE_JA != none; then LC_ALL=$LOCALE_JA \ ./test-wcrtomb${EXEEXT} 3 \ || exit 1 fi # Test whether a specific GB18030 locale is installed. : ${LOCALE_ZH_CN=zh_CN.GB18030} if test $LOCALE_ZH_CN != none; then LC_ALL=$LOCALE_ZH_CN \ ./test-wcrtomb${EXEEXT} 4 \ || exit 1 fi exit 0 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-verify.sh0000755000175000017500000000130513004436756017614 00000000000000#!/bin/sh . "${srcdir=.}/init.sh" # We are not interested in triggering bugs in the compilers and tools # (such as gcc 4.3.1 on openSUSE 11.0). unset MALLOC_PERTURB_ # Rather than figure out how to invoke the compiler with the right # include path ourselves, we let make do it: (cd "$initial_cwd_" && rm -f test-verify.o \ && $MAKE test-verify.o >/dev/null 2>&1) \ || skip_ "cannot compile error-free" # Now, prove that we encounter all expected compilation failures: : >out : >err for i in 1 2 3 4 5; do (cd "$initial_cwd_" rm -f test-verify.o $MAKE CFLAGS=-DEXP_FAIL=$i test-verify.o) >>out 2>>err \ && { warn_ "compiler didn't detect verification failure $i"; fail=1; } done Exit $fail gnuastro-0.2.33-8a3b/bootstrapped/tests/time.in.h0000644000175000017500000002564613004436756016526 00000000000000/* A more-standard . Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* Don't get in the way of glibc when it includes time.h merely to declare a few standard symbols, rather than to declare all the symbols. (However, skip this for MinGW as it treats __need_time_t incompatibly.) Also, Solaris 8 eventually includes itself recursively; if that is happening, just include the system without adding our own declarations. */ #if (((defined __need_time_t || defined __need_clock_t \ || defined __need_timespec) \ && !defined __MINGW32__) \ || defined _@GUARD_PREFIX@_TIME_H) # @INCLUDE_NEXT@ @NEXT_TIME_H@ #else # define _@GUARD_PREFIX@_TIME_H # @INCLUDE_NEXT@ @NEXT_TIME_H@ /* NetBSD 5.0 mis-defines NULL. */ # include /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Some systems don't define struct timespec (e.g., AIX 4.1, Ultrix 4.3). Or they define it with the wrong member names or define it in (e.g., FreeBSD circa 1997). Stock Mingw prior to 3.0 does not define it, but the pthreads-win32 library defines it in . */ # if ! @TIME_H_DEFINES_STRUCT_TIMESPEC@ # if @SYS_TIME_H_DEFINES_STRUCT_TIMESPEC@ # include # elif @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ # include # elif @UNISTD_H_DEFINES_STRUCT_TIMESPEC@ # include # else # ifdef __cplusplus extern "C" { # endif # if !GNULIB_defined_struct_timespec # undef timespec # define timespec rpl_timespec struct timespec { time_t tv_sec; long int tv_nsec; }; # define GNULIB_defined_struct_timespec 1 # endif # ifdef __cplusplus } # endif # endif # endif # if !GNULIB_defined_struct_time_t_must_be_integral /* Per http://austingroupbugs.net/view.php?id=327, POSIX requires time_t to be an integer type, even though C99 permits floating point. We don't know of any implementation that uses floating point, and it is much easier to write code that doesn't have to worry about that corner case, so we force the issue. */ struct __time_t_must_be_integral { unsigned int __floating_time_t_unsupported : (time_t) 1; }; # define GNULIB_defined_struct_time_t_must_be_integral 1 # endif /* Sleep for at least RQTP seconds unless interrupted, If interrupted, return -1 and store the remaining time into RMTP. See . */ # if @GNULIB_NANOSLEEP@ # if @REPLACE_NANOSLEEP@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define nanosleep rpl_nanosleep # endif _GL_FUNCDECL_RPL (nanosleep, int, (struct timespec const *__rqtp, struct timespec *__rmtp) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (nanosleep, int, (struct timespec const *__rqtp, struct timespec *__rmtp)); # else # if ! @HAVE_NANOSLEEP@ _GL_FUNCDECL_SYS (nanosleep, int, (struct timespec const *__rqtp, struct timespec *__rmtp) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (nanosleep, int, (struct timespec const *__rqtp, struct timespec *__rmtp)); # endif _GL_CXXALIASWARN (nanosleep); # endif /* Return the 'time_t' representation of TP and normalize TP. */ # if @GNULIB_MKTIME@ # if @REPLACE_MKTIME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define mktime rpl_mktime # endif _GL_FUNCDECL_RPL (mktime, time_t, (struct tm *__tp) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mktime, time_t, (struct tm *__tp)); # else _GL_CXXALIAS_SYS (mktime, time_t, (struct tm *__tp)); # endif _GL_CXXALIASWARN (mktime); # endif /* Convert TIMER to RESULT, assuming local time and UTC respectively. See and . */ # if @GNULIB_TIME_R@ # if @REPLACE_LOCALTIME_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef localtime_r # define localtime_r rpl_localtime_r # endif _GL_FUNCDECL_RPL (localtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (localtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result)); # else # if ! @HAVE_DECL_LOCALTIME_R@ _GL_FUNCDECL_SYS (localtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (localtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result)); # endif # if @HAVE_DECL_LOCALTIME_R@ _GL_CXXALIASWARN (localtime_r); # endif # if @REPLACE_LOCALTIME_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef gmtime_r # define gmtime_r rpl_gmtime_r # endif _GL_FUNCDECL_RPL (gmtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (gmtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result)); # else # if ! @HAVE_DECL_LOCALTIME_R@ _GL_FUNCDECL_SYS (gmtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (gmtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result)); # endif # if @HAVE_DECL_LOCALTIME_R@ _GL_CXXALIASWARN (gmtime_r); # endif # endif /* Convert TIMER to RESULT, assuming local time and UTC respectively. See and . */ # if @GNULIB_GETTIMEOFDAY@ # if @REPLACE_LOCALTIME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef localtime # define localtime rpl_localtime # endif _GL_FUNCDECL_RPL (localtime, struct tm *, (time_t const *__timer) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (localtime, struct tm *, (time_t const *__timer)); # else _GL_CXXALIAS_SYS (localtime, struct tm *, (time_t const *__timer)); # endif _GL_CXXALIASWARN (localtime); # endif # if @GNULIB_GETTIMEOFDAY@ # if @REPLACE_GMTIME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef gmtime # define gmtime rpl_gmtime # endif _GL_FUNCDECL_RPL (gmtime, struct tm *, (time_t const *__timer) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (gmtime, struct tm *, (time_t const *__timer)); # else _GL_CXXALIAS_SYS (gmtime, struct tm *, (time_t const *__timer)); # endif _GL_CXXALIASWARN (gmtime); # endif /* Parse BUF as a time stamp, assuming FORMAT specifies its layout, and store the resulting broken-down time into TM. See . */ # if @GNULIB_STRPTIME@ # if ! @HAVE_STRPTIME@ _GL_FUNCDECL_SYS (strptime, char *, (char const *restrict __buf, char const *restrict __format, struct tm *restrict __tm) _GL_ARG_NONNULL ((1, 2, 3))); # endif _GL_CXXALIAS_SYS (strptime, char *, (char const *restrict __buf, char const *restrict __format, struct tm *restrict __tm)); _GL_CXXALIASWARN (strptime); # endif # if defined _GNU_SOURCE && @GNULIB_TIME_RZ@ && ! @HAVE_TIMEZONE_T@ typedef struct tm_zone *timezone_t; _GL_FUNCDECL_SYS (tzalloc, timezone_t, (char const *__name)); _GL_CXXALIAS_SYS (tzalloc, timezone_t, (char const *__name)); _GL_FUNCDECL_SYS (tzfree, void, (timezone_t __tz)); _GL_CXXALIAS_SYS (tzfree, void, (timezone_t __tz)); _GL_FUNCDECL_SYS (localtime_rz, struct tm *, (timezone_t __tz, time_t const *restrict __timer, struct tm *restrict __result) _GL_ARG_NONNULL ((2, 3))); _GL_CXXALIAS_SYS (localtime_rz, struct tm *, (timezone_t __tz, time_t const *restrict __timer, struct tm *restrict __result)); _GL_FUNCDECL_SYS (mktime_z, time_t, (timezone_t __tz, struct tm *restrict __result) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_SYS (mktime_z, time_t, (timezone_t __tz, struct tm *restrict __result)); # endif /* Convert TM to a time_t value, assuming UTC. */ # if @GNULIB_TIMEGM@ # if @REPLACE_TIMEGM@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef timegm # define timegm rpl_timegm # endif _GL_FUNCDECL_RPL (timegm, time_t, (struct tm *__tm) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (timegm, time_t, (struct tm *__tm)); # else # if ! @HAVE_TIMEGM@ _GL_FUNCDECL_SYS (timegm, time_t, (struct tm *__tm) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (timegm, time_t, (struct tm *__tm)); # endif _GL_CXXALIASWARN (timegm); # endif /* Encourage applications to avoid unsafe functions that can overrun buffers when given outlandish struct tm values. Portable applications should use strftime (or even sprintf) instead. */ # if defined GNULIB_POSIXCHECK # undef asctime _GL_WARN_ON_USE (asctime, "asctime can overrun buffers in some cases - " "better use strftime (or even sprintf) instead"); # endif # if defined GNULIB_POSIXCHECK # undef asctime_r _GL_WARN_ON_USE (asctime, "asctime_r can overrun buffers in some cases - " "better use strftime (or even sprintf) instead"); # endif # if defined GNULIB_POSIXCHECK # undef ctime _GL_WARN_ON_USE (asctime, "ctime can overrun buffers in some cases - " "better use strftime (or even sprintf) instead"); # endif # if defined GNULIB_POSIXCHECK # undef ctime_r _GL_WARN_ON_USE (asctime, "ctime_r can overrun buffers in some cases - " "better use strftime (or even sprintf) instead"); # endif #endif gnuastro-0.2.33-8a3b/bootstrapped/tests/test-init.sh0000755000175000017500000000463313004436755017261 00000000000000#!/bin/sh # Unit tests for init.sh # Copyright (C) 2011-2016 Free Software Foundation, Inc. # This file is part of the GNUlib Library. # # This program is free software: you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see . */ : ${srcdir=.} . "$srcdir/init.sh"; path_prepend_ . fail=0 test_compare() { touch empty || fail=1 echo xyz > in || fail=1 compare /dev/null /dev/null >out 2>err || fail=1 test -s out && fail_ "out not empty: $(cat out)" # "err" should be empty, too, but has "set -x" output when VERBOSE=yes case $- in *x*) ;; *) test -s err && fail_ "err not empty: $(cat err)";; esac compare /dev/null empty >out 2>err || fail=1 test -s out && fail_ "out not empty: $(cat out)" case $- in *x*) ;; *) test -s err && fail_ "err not empty: $(cat err)";; esac compare in in >out 2>err || fail=1 test -s out && fail_ "out not empty: $(cat out)" case $- in *x*) ;; *) test -s err && fail_ "err not empty: $(cat err)";; esac compare /dev/null in >out 2>err && fail=1 cat <<\EOF > exp diff -u /dev/null in --- /dev/null 1970-01-01 +++ in 1970-01-01 +xyz EOF compare exp out || fail=1 case $- in *x*) ;; *) test -s err && fail_ "err not empty: $(cat err)";; esac compare empty in >out 2>err && fail=1 # Compare against expected output only if compare is using diff -u. if grep @ out >/dev/null; then # Remove the TAB-date suffix on each --- and +++ line, # for both the expected and the actual output files. # Also remove the @@ line, since Solaris 5.10 and GNU diff formats differ: # -@@ -0,0 +1 @@ # +@@ -1,0 +1,1 @@ # Also, remove space after leading '+', since AIX 7.1 diff outputs a space. sed 's/ .*//;/^@@/d;s/^+ /+/' out > k && mv k out cat <<\EOF > exp --- empty +++ in +xyz EOF compare exp out || fail=1 fi case $- in *x*) ;; *) test -s err && fail_ "err not empty: $(cat err)";; esac } test_compare Exit $fail gnuastro-0.2.33-8a3b/bootstrapped/tests/init.sh0000644000175000017500000004663713004436755016313 00000000000000# source this file; set up for tests # Copyright (C) 2009-2016 Free Software Foundation, Inc. # This program is free software: you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation, either version 3 of the License, or # (at your option) any later version. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # You should have received a copy of the GNU General Public License # along with this program. If not, see . # Using this file in a test # ========================= # # The typical skeleton of a test looks like this: # # #!/bin/sh # . "${srcdir=.}/init.sh"; path_prepend_ . # Execute some commands. # Note that these commands are executed in a subdirectory, therefore you # need to prepend "../" to relative filenames in the build directory. # Note that the "path_prepend_ ." is useful only if the body of your # test invokes programs residing in the initial directory. # For example, if the programs you want to test are in src/, and this test # script is named tests/test-1, then you would use "path_prepend_ ../src", # or perhaps export PATH='$(abs_top_builddir)/src$(PATH_SEPARATOR)'"$$PATH" # to all tests via automake's TESTS_ENVIRONMENT. # Set the exit code 0 for success, 77 for skipped, or 1 or other for failure. # Use the skip_ and fail_ functions to print a diagnostic and then exit # with the corresponding exit code. # Exit $? # Executing a test that uses this file # ==================================== # # Running a single test: # $ make check TESTS=test-foo.sh # # Running a single test, with verbose output: # $ make check TESTS=test-foo.sh VERBOSE=yes # # Running a single test, with single-stepping: # 1. Go into a sub-shell: # $ bash # 2. Set relevant environment variables from TESTS_ENVIRONMENT in the # Makefile: # $ export srcdir=../../tests # this is an example # 3. Execute the commands from the test, copy&pasting them one by one: # $ . "$srcdir/init.sh"; path_prepend_ . # ... # 4. Finally # $ exit ME_=`expr "./$0" : '.*/\(.*\)$'` # We use a trap below for cleanup. This requires us to go through # hoops to get the right exit status transported through the handler. # So use 'Exit STATUS' instead of 'exit STATUS' inside of the tests. # Turn off errexit here so that we don't trip the bug with OSF1/Tru64 # sh inside this function. Exit () { set +e; (exit $1); exit $1; } # Print warnings (e.g., about skipped and failed tests) to this file number. # Override by defining to say, 9, in init.cfg, and putting say, # export ...ENVVAR_SETTINGS...; $(SHELL) 9>&2 # in the definition of TESTS_ENVIRONMENT in your tests/Makefile.am file. # This is useful when using automake's parallel tests mode, to print # the reason for skip/failure to console, rather than to the .log files. : ${stderr_fileno_=2} # Note that correct expansion of "$*" depends on IFS starting with ' '. # Always write the full diagnostic to stderr. # When stderr_fileno_ is not 2, also emit the first line of the # diagnostic to that file descriptor. warn_ () { # If IFS does not start with ' ', set it and emit the warning in a subshell. case $IFS in ' '*) printf '%s\n' "$*" >&2 test $stderr_fileno_ = 2 \ || { printf '%s\n' "$*" | sed 1q >&$stderr_fileno_ ; } ;; *) (IFS=' '; warn_ "$@");; esac } fail_ () { warn_ "$ME_: failed test: $@"; Exit 1; } skip_ () { warn_ "$ME_: skipped test: $@"; Exit 77; } fatal_ () { warn_ "$ME_: hard error: $@"; Exit 99; } framework_failure_ () { warn_ "$ME_: set-up failure: $@"; Exit 99; } # This is used to simplify checking of the return value # which is useful when ensuring a command fails as desired. # I.e., just doing `command ... &&fail=1` will not catch # a segfault in command for example. With this helper you # instead check an explicit exit code like # returns_ 1 command ... || fail returns_ () { # Disable tracing so it doesn't interfere with stderr of the wrapped command { set +x; } 2>/dev/null local exp_exit="$1" shift "$@" test $? -eq $exp_exit && ret_=0 || ret_=1 if test "$VERBOSE" = yes && test "$gl_set_x_corrupts_stderr_" = false; then set -x fi { return $ret_; } 2>/dev/null } # Sanitize this shell to POSIX mode, if possible. DUALCASE=1; export DUALCASE if test -n "${ZSH_VERSION+set}" && (emulate sh) >/dev/null 2>&1; then emulate sh NULLCMD=: alias -g '${1+"$@"}'='"$@"' setopt NO_GLOB_SUBST else case `(set -o) 2>/dev/null` in *posix*) set -o posix ;; esac fi # We require $(...) support unconditionally. # We require non-surprising "local" semantics (this eliminates dash). # This takes the admittedly draconian step of eliminating dash, because the # assignment tab=$(printf '\t') works fine, yet preceding it with "local " # transforms it into an assignment that sets the variable to the empty string. # That is too counter-intuitive, and can lead to subtle run-time malfunction. # The example below is less subtle in that with dash, it evokes the run-time # exception "dash: 1: local: 1: bad variable name". # We require a few additional shell features only when $EXEEXT is nonempty, # in order to support automatic $EXEEXT emulation: # - hyphen-containing alias names # - we prefer to use ${var#...} substitution, rather than having # to work around lack of support for that feature. # The following code attempts to find a shell with support for these features. # If the current shell passes the test, we're done. Otherwise, test other # shells until we find one that passes. If one is found, re-exec it. # If no acceptable shell is found, skip the current test. # # The "...set -x; P=1 true 2>err..." test is to disqualify any shell that # emits "P=1" into err, as /bin/sh from SunOS 5.11 and OpenBSD 4.7 do. # # Use "9" to indicate success (rather than 0), in case some shell acts # like Solaris 10's /bin/sh but exits successfully instead of with status 2. # Eval this code in a subshell to determine a shell's suitability. # 10 - passes all tests; ok to use # 9 - ok, but enabling "set -x" corrupts app stderr; prefer higher score # ? - not ok gl_shell_test_script_=' test $(echo y) = y || exit 1 f_local_() { local v=1; }; f_local_ || exit 1 f_dash_local_fail_() { local t=$(printf " 1"); }; f_dash_local_fail_ score_=10 if test "$VERBOSE" = yes; then test -n "$( (exec 3>&1; set -x; P=1 true 2>&3) 2> /dev/null)" && score_=9 fi test -z "$EXEEXT" && exit $score_ shopt -s expand_aliases alias a-b="echo zoo" v=abx test ${v%x} = ab \ && test ${v#a} = bx \ && test $(a-b) = zoo \ && exit $score_ ' if test "x$1" = "x--no-reexec"; then shift else # Assume a working shell. Export to subshells (setup_ needs this). gl_set_x_corrupts_stderr_=false export gl_set_x_corrupts_stderr_ # Record the first marginally acceptable shell. marginal_= # Search for a shell that meets our requirements. for re_shell_ in __current__ "${CONFIG_SHELL:-no_shell}" \ /bin/sh bash dash zsh pdksh fail do test "$re_shell_" = no_shell && continue # If we've made it all the way to the sentinel, "fail" without # finding even a marginal shell, skip this test. if test "$re_shell_" = fail; then test -z "$marginal_" && skip_ failed to find an adequate shell re_shell_=$marginal_ break fi # When testing the current shell, simply "eval" the test code. # Otherwise, run it via $re_shell_ -c ... if test "$re_shell_" = __current__; then # 'eval'ing this code makes Solaris 10's /bin/sh exit with # $? set to 2. It does not evaluate any of the code after the # "unexpected" first '('. Thus, we must run it in a subshell. ( eval "$gl_shell_test_script_" ) > /dev/null 2>&1 else "$re_shell_" -c "$gl_shell_test_script_" 2>/dev/null fi st_=$? # $re_shell_ works just fine. Use it. if test $st_ = 10; then gl_set_x_corrupts_stderr_=false break fi # If this is our first marginally acceptable shell, remember it. if test "$st_:$marginal_" = 9: ; then marginal_="$re_shell_" gl_set_x_corrupts_stderr_=true fi done if test "$re_shell_" != __current__; then # Found a usable shell. Preserve -v and -x. case $- in *v*x* | *x*v*) opts_=-vx ;; *v*) opts_=-v ;; *x*) opts_=-x ;; *) opts_= ;; esac re_shell=$re_shell_ export re_shell exec "$re_shell_" $opts_ "$0" --no-reexec "$@" echo "$ME_: exec failed" 1>&2 exit 127 fi fi # If this is bash, turn off all aliases. test -n "$BASH_VERSION" && unalias -a # Note that when supporting $EXEEXT (transparently mapping from PROG_NAME to # PROG_NAME.exe), we want to support hyphen-containing names like test-acos. # That is part of the shell-selection test above. Why use aliases rather # than functions? Because support for hyphen-containing aliases is more # widespread than that for hyphen-containing function names. test -n "$EXEEXT" && shopt -s expand_aliases # Enable glibc's malloc-perturbing option. # This is useful for exposing code that depends on the fact that # malloc-related functions often return memory that is mostly zeroed. # If you have the time and cycles, use valgrind to do an even better job. : ${MALLOC_PERTURB_=87} export MALLOC_PERTURB_ # This is a stub function that is run upon trap (upon regular exit and # interrupt). Override it with a per-test function, e.g., to unmount # a partition, or to undo any other global state changes. cleanup_ () { :; } # Emit a header similar to that from diff -u; Print the simulated "diff" # command so that the order of arguments is clear. Don't bother with @@ lines. emit_diff_u_header_ () { printf '%s\n' "diff -u $*" \ "--- $1 1970-01-01" \ "+++ $2 1970-01-01" } # Arrange not to let diff or cmp operate on /dev/null, # since on some systems (at least OSF/1 5.1), that doesn't work. # When there are not two arguments, or no argument is /dev/null, return 2. # When one argument is /dev/null and the other is not empty, # cat the nonempty file to stderr and return 1. # Otherwise, return 0. compare_dev_null_ () { test $# = 2 || return 2 if test "x$1" = x/dev/null; then test -s "$2" || return 0 emit_diff_u_header_ "$@"; sed 's/^/+/' "$2" return 1 fi if test "x$2" = x/dev/null; then test -s "$1" || return 0 emit_diff_u_header_ "$@"; sed 's/^/-/' "$1" return 1 fi return 2 } for diff_opt_ in -u -U3 -c '' no; do test "$diff_opt_" != no && diff_out_=`exec 2>/dev/null; diff $diff_opt_ "$0" "$0" < /dev/null` && break done if test "$diff_opt_" != no; then if test -z "$diff_out_"; then compare_ () { diff $diff_opt_ "$@"; } else compare_ () { # If no differences were found, AIX and HP-UX 'diff' produce output # like "No differences encountered". Hide this output. diff $diff_opt_ "$@" > diff.out diff_status_=$? test $diff_status_ -eq 0 || cat diff.out || diff_status_=2 rm -f diff.out || diff_status_=2 return $diff_status_ } fi elif cmp -s /dev/null /dev/null 2>/dev/null; then compare_ () { cmp -s "$@"; } else compare_ () { cmp "$@"; } fi # Usage: compare EXPECTED ACTUAL # # Given compare_dev_null_'s preprocessing, defer to compare_ if 2 or more. # Otherwise, propagate $? to caller: any diffs have already been printed. compare () { # This looks like it can be factored to use a simple "case $?" # after unchecked compare_dev_null_ invocation, but that would # fail in a "set -e" environment. if compare_dev_null_ "$@"; then return 0 else case $? in 1) return 1;; *) compare_ "$@";; esac fi } # An arbitrary prefix to help distinguish test directories. testdir_prefix_ () { printf gt; } # Run the user-overridable cleanup_ function, remove the temporary # directory and exit with the incoming value of $?. remove_tmp_ () { __st=$? cleanup_ # cd out of the directory we're about to remove cd "$initial_cwd_" || cd / || cd /tmp chmod -R u+rwx "$test_dir_" # If removal fails and exit status was to be 0, then change it to 1. rm -rf "$test_dir_" || { test $__st = 0 && __st=1; } exit $__st } # Given a directory name, DIR, if every entry in it that matches *.exe # contains only the specified bytes (see the case stmt below), then print # a space-separated list of those names and return 0. Otherwise, don't # print anything and return 1. Naming constraints apply also to DIR. find_exe_basenames_ () { feb_dir_=$1 feb_fail_=0 feb_result_= feb_sp_= for feb_file_ in $feb_dir_/*.exe; do # If there was no *.exe file, or there existed a file named "*.exe" that # was deleted between the above glob expansion and the existence test # below, just skip it. test "x$feb_file_" = "x$feb_dir_/*.exe" && test ! -f "$feb_file_" \ && continue # Exempt [.exe, since we can't create a function by that name, yet # we can't invoke [ by PATH search anyways due to shell builtins. test "x$feb_file_" = "x$feb_dir_/[.exe" && continue case $feb_file_ in *[!-a-zA-Z/0-9_.+]*) feb_fail_=1; break;; *) # Remove leading file name components as well as the .exe suffix. feb_file_=${feb_file_##*/} feb_file_=${feb_file_%.exe} feb_result_="$feb_result_$feb_sp_$feb_file_";; esac feb_sp_=' ' done test $feb_fail_ = 0 && printf %s "$feb_result_" return $feb_fail_ } # Consider the files in directory, $1. # For each file name of the form PROG.exe, create an alias named # PROG that simply invokes PROG.exe, then return 0. If any selected # file name or the directory name, $1, contains an unexpected character, # define no alias and return 1. create_exe_shims_ () { case $EXEEXT in '') return 0 ;; .exe) ;; *) echo "$0: unexpected \$EXEEXT value: $EXEEXT" 1>&2; return 1 ;; esac base_names_=`find_exe_basenames_ $1` \ || { echo "$0 (exe_shim): skipping directory: $1" 1>&2; return 0; } if test -n "$base_names_"; then for base_ in $base_names_; do alias "$base_"="$base_$EXEEXT" done fi return 0 } # Use this function to prepend to PATH an absolute name for each # specified, possibly-$initial_cwd_-relative, directory. path_prepend_ () { while test $# != 0; do path_dir_=$1 case $path_dir_ in '') fail_ "invalid path dir: '$1'";; /*) abs_path_dir_=$path_dir_;; *) abs_path_dir_=$initial_cwd_/$path_dir_;; esac case $abs_path_dir_ in *:*) fail_ "invalid path dir: '$abs_path_dir_'";; esac PATH="$abs_path_dir_:$PATH" # Create an alias, FOO, for each FOO.exe in this directory. create_exe_shims_ "$abs_path_dir_" \ || fail_ "something failed (above): $abs_path_dir_" shift done export PATH } setup_ () { if test "$VERBOSE" = yes; then # Test whether set -x may cause the selected shell to corrupt an # application's stderr. Many do, including zsh-4.3.10 and the /bin/sh # from SunOS 5.11, OpenBSD 4.7 and Irix 5.x and 6.5. # If enabling verbose output this way would cause trouble, simply # issue a warning and refrain. if $gl_set_x_corrupts_stderr_; then warn_ "using SHELL=$SHELL with 'set -x' corrupts stderr" else set -x fi fi initial_cwd_=$PWD pfx_=`testdir_prefix_` test_dir_=`mktempd_ "$initial_cwd_" "$pfx_-$ME_.XXXX"` \ || fail_ "failed to create temporary directory in $initial_cwd_" cd "$test_dir_" || fail_ "failed to cd to temporary directory" # As autoconf-generated configure scripts do, ensure that IFS # is defined initially, so that saving and restoring $IFS works. gl_init_sh_nl_=' ' IFS=" "" $gl_init_sh_nl_" # This trap statement, along with a trap on 0 below, ensure that the # temporary directory, $test_dir_, is removed upon exit as well as # upon receipt of any of the listed signals. for sig_ in 1 2 3 13 15; do eval "trap 'Exit $(expr $sig_ + 128)' $sig_" done } # Create a temporary directory, much like mktemp -d does. # Written by Jim Meyering. # # Usage: mktempd_ /tmp phoey.XXXXXXXXXX # # First, try to use the mktemp program. # Failing that, we'll roll our own mktemp-like function: # - try to get random bytes from /dev/urandom # - failing that, generate output from a combination of quickly-varying # sources and gzip. Ignore non-varying gzip header, and extract # "random" bits from there. # - given those bits, map to file-name bytes using tr, and try to create # the desired directory. # - make only $MAX_TRIES_ attempts # Helper function. Print $N pseudo-random bytes from a-zA-Z0-9. rand_bytes_ () { n_=$1 # Maybe try openssl rand -base64 $n_prime_|tr '+/=\012' abcd first? # But if they have openssl, they probably have mktemp, too. chars_=abcdefghijklmnopqrstuvwxyzABCDEFGHIJKLMNOPQRSTUVWXYZ0123456789 dev_rand_=/dev/urandom if test -r "$dev_rand_"; then # Note: 256-length($chars_) == 194; 3 copies of $chars_ is 186 + 8 = 194. dd ibs=$n_ count=1 if=$dev_rand_ 2>/dev/null \ | LC_ALL=C tr -c $chars_ 01234567$chars_$chars_$chars_ return fi n_plus_50_=`expr $n_ + 50` cmds_='date; date +%N; free; who -a; w; ps auxww; ps ef; netstat -n' data_=` (eval "$cmds_") 2>&1 | gzip ` # Ensure that $data_ has length at least 50+$n_ while :; do len_=`echo "$data_"|wc -c` test $n_plus_50_ -le $len_ && break; data_=` (echo "$data_"; eval "$cmds_") 2>&1 | gzip ` done echo "$data_" \ | dd bs=1 skip=50 count=$n_ 2>/dev/null \ | LC_ALL=C tr -c $chars_ 01234567$chars_$chars_$chars_ } mktempd_ () { case $# in 2);; *) fail_ "Usage: mktempd_ DIR TEMPLATE";; esac destdir_=$1 template_=$2 MAX_TRIES_=4 # Disallow any trailing slash on specified destdir: # it would subvert the post-mktemp "case"-based destdir test. case $destdir_ in / | //) destdir_slash_=$destdir;; */) fail_ "invalid destination dir: remove trailing slash(es)";; *) destdir_slash_=$destdir_/;; esac case $template_ in *XXXX) ;; *) fail_ \ "invalid template: $template_ (must have a suffix of at least 4 X's)";; esac # First, try to use mktemp. d=`unset TMPDIR; { mktemp -d -t -p "$destdir_" "$template_"; } 2>/dev/null` && # The resulting name must be in the specified directory. case $d in "$destdir_slash_"*) :;; *) false;; esac && # It must have created the directory. test -d "$d" && # It must have 0700 permissions. Handle sticky "S" bits. perms=`ls -dgo "$d" 2>/dev/null` && case $perms in drwx--[-S]---*) :;; *) false;; esac && { echo "$d" return } # If we reach this point, we'll have to create a directory manually. # Get a copy of the template without its suffix of X's. base_template_=`echo "$template_"|sed 's/XX*$//'` # Calculate how many X's we've just removed. template_length_=`echo "$template_" | wc -c` nx_=`echo "$base_template_" | wc -c` nx_=`expr $template_length_ - $nx_` err_= i_=1 while :; do X_=`rand_bytes_ $nx_` candidate_dir_="$destdir_slash_$base_template_$X_" err_=`mkdir -m 0700 "$candidate_dir_" 2>&1` \ && { echo "$candidate_dir_"; return; } test $MAX_TRIES_ -le $i_ && break; i_=`expr $i_ + 1` done fail_ "$err_" } # If you want to override the testdir_prefix_ function, # or to add more utility functions, use this file. test -f "$srcdir/init.cfg" \ && . "$srcdir/init.cfg" setup_ "$@" # This trap is here, rather than in the setup_ function, because some # shells run the exit trap at shell function exit, rather than script exit. trap remove_tmp_ 0 gnuastro-0.2.33-8a3b/bootstrapped/tests/sys_time.in.h0000644000175000017500000001700113004436755017405 00000000000000/* Provide a more complete sys/time.h. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Paul Eggert. */ #ifndef _@GUARD_PREFIX@_SYS_TIME_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* On Cygwin and on many BSDish systems, includes itself recursively via . Simply delegate to the system's header in this case; it is a no-op. Without this extra ifdef, the C++ gettimeofday declaration below would be a forward declaration in gnulib's nested . */ #if defined _CYGWIN_SYS_TIME_H || defined _SYS_TIME_H || defined _SYS_TIME_H_ # @INCLUDE_NEXT@ @NEXT_SYS_TIME_H@ #else /* The include_next requires a split double-inclusion guard. */ #if @HAVE_SYS_TIME_H@ # @INCLUDE_NEXT@ @NEXT_SYS_TIME_H@ #endif #ifndef _@GUARD_PREFIX@_SYS_TIME_H #define _@GUARD_PREFIX@_SYS_TIME_H #if ! @HAVE_SYS_TIME_H@ # include #endif /* On native Windows with MSVC, get the 'struct timeval' type. Also, on native Windows with a 64-bit time_t, where we are overriding the 'struct timeval' type, get all declarations of system functions whose signature contains 'struct timeval'. */ #if (defined _MSC_VER || @REPLACE_STRUCT_TIMEVAL@) && @HAVE_WINSOCK2_H@ && !defined _GL_INCLUDING_WINSOCK2_H # define _GL_INCLUDING_WINSOCK2_H # include # undef _GL_INCLUDING_WINSOCK2_H #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ #ifdef __cplusplus extern "C" { #endif #if !@HAVE_STRUCT_TIMEVAL@ || @REPLACE_STRUCT_TIMEVAL@ # if @REPLACE_STRUCT_TIMEVAL@ # define timeval rpl_timeval # endif # if !GNULIB_defined_struct_timeval struct timeval { time_t tv_sec; long int tv_usec; }; # define GNULIB_defined_struct_timeval 1 # endif #endif #ifdef __cplusplus } #endif #if @GNULIB_GETTIMEOFDAY@ # if @REPLACE_GETTIMEOFDAY@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef gettimeofday # define gettimeofday rpl_gettimeofday # endif _GL_FUNCDECL_RPL (gettimeofday, int, (struct timeval *restrict, void *restrict) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (gettimeofday, int, (struct timeval *restrict, void *restrict)); # else # if !@HAVE_GETTIMEOFDAY@ _GL_FUNCDECL_SYS (gettimeofday, int, (struct timeval *restrict, void *restrict) _GL_ARG_NONNULL ((1))); # endif /* Need to cast, because on glibc systems, by default, the second argument is struct timezone *. */ _GL_CXXALIAS_SYS_CAST (gettimeofday, int, (struct timeval *restrict, void *restrict)); # endif _GL_CXXALIASWARN (gettimeofday); #elif defined GNULIB_POSIXCHECK # undef gettimeofday # if HAVE_RAW_DECL_GETTIMEOFDAY _GL_WARN_ON_USE (gettimeofday, "gettimeofday is unportable - " "use gnulib module gettimeofday for portability"); # endif #endif /* Hide some function declarations from . */ #if defined _MSC_VER && @HAVE_WINSOCK2_H@ # if !defined _@GUARD_PREFIX@_UNISTD_H # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef close # define close close_used_without_including_unistd_h # else _GL_WARN_ON_USE (close, "close() used without including "); # endif # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef gethostname # define gethostname gethostname_used_without_including_unistd_h # else _GL_WARN_ON_USE (gethostname, "gethostname() used without including "); # endif # endif # if !defined _@GUARD_PREFIX@_SYS_SOCKET_H # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef socket # define socket socket_used_without_including_sys_socket_h # undef connect # define connect connect_used_without_including_sys_socket_h # undef accept # define accept accept_used_without_including_sys_socket_h # undef bind # define bind bind_used_without_including_sys_socket_h # undef getpeername # define getpeername getpeername_used_without_including_sys_socket_h # undef getsockname # define getsockname getsockname_used_without_including_sys_socket_h # undef getsockopt # define getsockopt getsockopt_used_without_including_sys_socket_h # undef listen # define listen listen_used_without_including_sys_socket_h # undef recv # define recv recv_used_without_including_sys_socket_h # undef send # define send send_used_without_including_sys_socket_h # undef recvfrom # define recvfrom recvfrom_used_without_including_sys_socket_h # undef sendto # define sendto sendto_used_without_including_sys_socket_h # undef setsockopt # define setsockopt setsockopt_used_without_including_sys_socket_h # undef shutdown # define shutdown shutdown_used_without_including_sys_socket_h # else _GL_WARN_ON_USE (socket, "socket() used without including "); _GL_WARN_ON_USE (connect, "connect() used without including "); _GL_WARN_ON_USE (accept, "accept() used without including "); _GL_WARN_ON_USE (bind, "bind() used without including "); _GL_WARN_ON_USE (getpeername, "getpeername() used without including "); _GL_WARN_ON_USE (getsockname, "getsockname() used without including "); _GL_WARN_ON_USE (getsockopt, "getsockopt() used without including "); _GL_WARN_ON_USE (listen, "listen() used without including "); _GL_WARN_ON_USE (recv, "recv() used without including "); _GL_WARN_ON_USE (send, "send() used without including "); _GL_WARN_ON_USE (recvfrom, "recvfrom() used without including "); _GL_WARN_ON_USE (sendto, "sendto() used without including "); _GL_WARN_ON_USE (setsockopt, "setsockopt() used without including "); _GL_WARN_ON_USE (shutdown, "shutdown() used without including "); # endif # endif # if !defined _@GUARD_PREFIX@_SYS_SELECT_H # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef select # define select select_used_without_including_sys_select_h # else _GL_WARN_ON_USE (select, "select() used without including "); # endif # endif #endif #endif /* _@GUARD_PREFIX@_SYS_TIME_H */ #endif /* _CYGWIN_SYS_TIME_H */ #endif /* _@GUARD_PREFIX@_SYS_TIME_H */ gnuastro-0.2.33-8a3b/bootstrapped/tests/sys_stat.in.h0000644000175000017500000004767113004436755017442 00000000000000/* Provide a more complete sys/stat header file. Copyright (C) 2005-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Eric Blake, Paul Eggert, and Jim Meyering. */ /* This file is supposed to be used on platforms where is incomplete. It is intended to provide definitions and prototypes needed by an application. Start with what the system provides. */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if defined __need_system_sys_stat_h /* Special invocation convention. */ #@INCLUDE_NEXT@ @NEXT_SYS_STAT_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_SYS_STAT_H /* Get nlink_t. May also define off_t to a 64-bit type on native Windows. */ #include /* Get struct timespec. */ #include /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_SYS_STAT_H@ #ifndef _@GUARD_PREFIX@_SYS_STAT_H #define _@GUARD_PREFIX@_SYS_STAT_H /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Before doing "#define mkdir rpl_mkdir" below, we need to include all headers that may declare mkdir(). Native Windows platforms declare mkdir in and/or , not in . */ #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # include /* mingw32, mingw64 */ # include /* mingw64, MSVC 9 */ #endif /* Native Windows platforms declare umask() in . */ #if 0 && ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) # include #endif /* Large File Support on native Windows. */ #if @WINDOWS_64_BIT_ST_SIZE@ # define stat _stati64 #endif #ifndef S_IFIFO # ifdef _S_IFIFO # define S_IFIFO _S_IFIFO # endif #endif #ifndef S_IFMT # define S_IFMT 0170000 #endif #if STAT_MACROS_BROKEN # undef S_ISBLK # undef S_ISCHR # undef S_ISDIR # undef S_ISFIFO # undef S_ISLNK # undef S_ISNAM # undef S_ISMPB # undef S_ISMPC # undef S_ISNWK # undef S_ISREG # undef S_ISSOCK #endif #ifndef S_ISBLK # ifdef S_IFBLK # define S_ISBLK(m) (((m) & S_IFMT) == S_IFBLK) # else # define S_ISBLK(m) 0 # endif #endif #ifndef S_ISCHR # ifdef S_IFCHR # define S_ISCHR(m) (((m) & S_IFMT) == S_IFCHR) # else # define S_ISCHR(m) 0 # endif #endif #ifndef S_ISDIR # ifdef S_IFDIR # define S_ISDIR(m) (((m) & S_IFMT) == S_IFDIR) # else # define S_ISDIR(m) 0 # endif #endif #ifndef S_ISDOOR /* Solaris 2.5 and up */ # define S_ISDOOR(m) 0 #endif #ifndef S_ISFIFO # ifdef S_IFIFO # define S_ISFIFO(m) (((m) & S_IFMT) == S_IFIFO) # else # define S_ISFIFO(m) 0 # endif #endif #ifndef S_ISLNK # ifdef S_IFLNK # define S_ISLNK(m) (((m) & S_IFMT) == S_IFLNK) # else # define S_ISLNK(m) 0 # endif #endif #ifndef S_ISMPB /* V7 */ # ifdef S_IFMPB # define S_ISMPB(m) (((m) & S_IFMT) == S_IFMPB) # define S_ISMPC(m) (((m) & S_IFMT) == S_IFMPC) # else # define S_ISMPB(m) 0 # define S_ISMPC(m) 0 # endif #endif #ifndef S_ISMPX /* AIX */ # define S_ISMPX(m) 0 #endif #ifndef S_ISNAM /* Xenix */ # ifdef S_IFNAM # define S_ISNAM(m) (((m) & S_IFMT) == S_IFNAM) # else # define S_ISNAM(m) 0 # endif #endif #ifndef S_ISNWK /* HP/UX */ # ifdef S_IFNWK # define S_ISNWK(m) (((m) & S_IFMT) == S_IFNWK) # else # define S_ISNWK(m) 0 # endif #endif #ifndef S_ISPORT /* Solaris 10 and up */ # define S_ISPORT(m) 0 #endif #ifndef S_ISREG # ifdef S_IFREG # define S_ISREG(m) (((m) & S_IFMT) == S_IFREG) # else # define S_ISREG(m) 0 # endif #endif #ifndef S_ISSOCK # ifdef S_IFSOCK # define S_ISSOCK(m) (((m) & S_IFMT) == S_IFSOCK) # else # define S_ISSOCK(m) 0 # endif #endif #ifndef S_TYPEISMQ # define S_TYPEISMQ(p) 0 #endif #ifndef S_TYPEISTMO # define S_TYPEISTMO(p) 0 #endif #ifndef S_TYPEISSEM # ifdef S_INSEM # define S_TYPEISSEM(p) (S_ISNAM ((p)->st_mode) && (p)->st_rdev == S_INSEM) # else # define S_TYPEISSEM(p) 0 # endif #endif #ifndef S_TYPEISSHM # ifdef S_INSHD # define S_TYPEISSHM(p) (S_ISNAM ((p)->st_mode) && (p)->st_rdev == S_INSHD) # else # define S_TYPEISSHM(p) 0 # endif #endif /* high performance ("contiguous data") */ #ifndef S_ISCTG # define S_ISCTG(p) 0 #endif /* Cray DMF (data migration facility): off line, with data */ #ifndef S_ISOFD # define S_ISOFD(p) 0 #endif /* Cray DMF (data migration facility): off line, with no data */ #ifndef S_ISOFL # define S_ISOFL(p) 0 #endif /* 4.4BSD whiteout */ #ifndef S_ISWHT # define S_ISWHT(m) 0 #endif /* If any of the following are undefined, define them to their de facto standard values. */ #if !S_ISUID # define S_ISUID 04000 #endif #if !S_ISGID # define S_ISGID 02000 #endif /* S_ISVTX is a common extension to POSIX. */ #ifndef S_ISVTX # define S_ISVTX 01000 #endif #if !S_IRUSR && S_IREAD # define S_IRUSR S_IREAD #endif #if !S_IRUSR # define S_IRUSR 00400 #endif #if !S_IRGRP # define S_IRGRP (S_IRUSR >> 3) #endif #if !S_IROTH # define S_IROTH (S_IRUSR >> 6) #endif #if !S_IWUSR && S_IWRITE # define S_IWUSR S_IWRITE #endif #if !S_IWUSR # define S_IWUSR 00200 #endif #if !S_IWGRP # define S_IWGRP (S_IWUSR >> 3) #endif #if !S_IWOTH # define S_IWOTH (S_IWUSR >> 6) #endif #if !S_IXUSR && S_IEXEC # define S_IXUSR S_IEXEC #endif #if !S_IXUSR # define S_IXUSR 00100 #endif #if !S_IXGRP # define S_IXGRP (S_IXUSR >> 3) #endif #if !S_IXOTH # define S_IXOTH (S_IXUSR >> 6) #endif #if !S_IRWXU # define S_IRWXU (S_IRUSR | S_IWUSR | S_IXUSR) #endif #if !S_IRWXG # define S_IRWXG (S_IRGRP | S_IWGRP | S_IXGRP) #endif #if !S_IRWXO # define S_IRWXO (S_IROTH | S_IWOTH | S_IXOTH) #endif /* S_IXUGO is a common extension to POSIX. */ #if !S_IXUGO # define S_IXUGO (S_IXUSR | S_IXGRP | S_IXOTH) #endif #ifndef S_IRWXUGO # define S_IRWXUGO (S_IRWXU | S_IRWXG | S_IRWXO) #endif /* Macros for futimens and utimensat. */ #ifndef UTIME_NOW # define UTIME_NOW (-1) # define UTIME_OMIT (-2) #endif #if @GNULIB_FCHMODAT@ # if !@HAVE_FCHMODAT@ _GL_FUNCDECL_SYS (fchmodat, int, (int fd, char const *file, mode_t mode, int flag) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (fchmodat, int, (int fd, char const *file, mode_t mode, int flag)); _GL_CXXALIASWARN (fchmodat); #elif defined GNULIB_POSIXCHECK # undef fchmodat # if HAVE_RAW_DECL_FCHMODAT _GL_WARN_ON_USE (fchmodat, "fchmodat is not portable - " "use gnulib module openat for portability"); # endif #endif #if @GNULIB_FSTAT@ # if @REPLACE_FSTAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fstat # define fstat rpl_fstat # endif _GL_FUNCDECL_RPL (fstat, int, (int fd, struct stat *buf) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (fstat, int, (int fd, struct stat *buf)); # else _GL_CXXALIAS_SYS (fstat, int, (int fd, struct stat *buf)); # endif _GL_CXXALIASWARN (fstat); #elif @WINDOWS_64_BIT_ST_SIZE@ /* Above, we define stat to _stati64. */ # define fstat _fstati64 #elif defined GNULIB_POSIXCHECK # undef fstat # if HAVE_RAW_DECL_FSTAT _GL_WARN_ON_USE (fstat, "fstat has portability problems - " "use gnulib module fstat for portability"); # endif #endif #if @GNULIB_FSTATAT@ # if @REPLACE_FSTATAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fstatat # define fstatat rpl_fstatat # endif _GL_FUNCDECL_RPL (fstatat, int, (int fd, char const *name, struct stat *st, int flags) _GL_ARG_NONNULL ((2, 3))); _GL_CXXALIAS_RPL (fstatat, int, (int fd, char const *name, struct stat *st, int flags)); # else # if !@HAVE_FSTATAT@ _GL_FUNCDECL_SYS (fstatat, int, (int fd, char const *name, struct stat *st, int flags) _GL_ARG_NONNULL ((2, 3))); # endif _GL_CXXALIAS_SYS (fstatat, int, (int fd, char const *name, struct stat *st, int flags)); # endif _GL_CXXALIASWARN (fstatat); #elif defined GNULIB_POSIXCHECK # undef fstatat # if HAVE_RAW_DECL_FSTATAT _GL_WARN_ON_USE (fstatat, "fstatat is not portable - " "use gnulib module openat for portability"); # endif #endif #if @GNULIB_FUTIMENS@ /* Use the rpl_ prefix also on Solaris <= 9, because on Solaris 9 our futimens implementation relies on futimesat, which on Solaris 10 makes an invocation to futimens that is meant to invoke the libc's futimens(), not gnulib's futimens(). */ # if @REPLACE_FUTIMENS@ || (!@HAVE_FUTIMENS@ && defined __sun) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef futimens # define futimens rpl_futimens # endif _GL_FUNCDECL_RPL (futimens, int, (int fd, struct timespec const times[2])); _GL_CXXALIAS_RPL (futimens, int, (int fd, struct timespec const times[2])); # else # if !@HAVE_FUTIMENS@ _GL_FUNCDECL_SYS (futimens, int, (int fd, struct timespec const times[2])); # endif _GL_CXXALIAS_SYS (futimens, int, (int fd, struct timespec const times[2])); # endif # if @HAVE_FUTIMENS@ _GL_CXXALIASWARN (futimens); # endif #elif defined GNULIB_POSIXCHECK # undef futimens # if HAVE_RAW_DECL_FUTIMENS _GL_WARN_ON_USE (futimens, "futimens is not portable - " "use gnulib module futimens for portability"); # endif #endif #if @GNULIB_LCHMOD@ /* Change the mode of FILENAME to MODE, without dereferencing it if FILENAME denotes a symbolic link. */ # if !@HAVE_LCHMOD@ /* The lchmod replacement follows symbolic links. Callers should take this into account; lchmod should be applied only to arguments that are known to not be symbolic links. On hosts that lack lchmod, this can lead to race conditions between the check and the invocation of lchmod, but we know of no workarounds that are reliable in general. You might try requesting support for lchmod from your operating system supplier. */ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define lchmod chmod # endif /* Need to cast, because on mingw, the second parameter of chmod is int mode. */ _GL_CXXALIAS_RPL_CAST_1 (lchmod, chmod, int, (const char *filename, mode_t mode)); # else # if 0 /* assume already declared */ _GL_FUNCDECL_SYS (lchmod, int, (const char *filename, mode_t mode) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (lchmod, int, (const char *filename, mode_t mode)); # endif # if @HAVE_LCHMOD@ _GL_CXXALIASWARN (lchmod); # endif #elif defined GNULIB_POSIXCHECK # undef lchmod # if HAVE_RAW_DECL_LCHMOD _GL_WARN_ON_USE (lchmod, "lchmod is unportable - " "use gnulib module lchmod for portability"); # endif #endif #if @GNULIB_LSTAT@ # if ! @HAVE_LSTAT@ /* mingw does not support symlinks, therefore it does not have lstat. But without links, stat does just fine. */ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define lstat stat # endif _GL_CXXALIAS_RPL_1 (lstat, stat, int, (const char *name, struct stat *buf)); # elif @REPLACE_LSTAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef lstat # define lstat rpl_lstat # endif _GL_FUNCDECL_RPL (lstat, int, (const char *name, struct stat *buf) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (lstat, int, (const char *name, struct stat *buf)); # else _GL_CXXALIAS_SYS (lstat, int, (const char *name, struct stat *buf)); # endif # if @HAVE_LSTAT@ _GL_CXXALIASWARN (lstat); # endif #elif defined GNULIB_POSIXCHECK # undef lstat # if HAVE_RAW_DECL_LSTAT _GL_WARN_ON_USE (lstat, "lstat is unportable - " "use gnulib module lstat for portability"); # endif #endif #if @REPLACE_MKDIR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mkdir # define mkdir rpl_mkdir # endif _GL_FUNCDECL_RPL (mkdir, int, (char const *name, mode_t mode) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mkdir, int, (char const *name, mode_t mode)); #else /* mingw's _mkdir() function has 1 argument, but we pass 2 arguments. Additionally, it declares _mkdir (and depending on compile flags, an alias mkdir), only in the nonstandard includes and , which are included above. */ # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # if !GNULIB_defined_rpl_mkdir static int rpl_mkdir (char const *name, mode_t mode) { return _mkdir (name); } # define GNULIB_defined_rpl_mkdir 1 # endif # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define mkdir rpl_mkdir # endif _GL_CXXALIAS_RPL (mkdir, int, (char const *name, mode_t mode)); # else _GL_CXXALIAS_SYS (mkdir, int, (char const *name, mode_t mode)); # endif #endif _GL_CXXALIASWARN (mkdir); #if @GNULIB_MKDIRAT@ # if !@HAVE_MKDIRAT@ _GL_FUNCDECL_SYS (mkdirat, int, (int fd, char const *file, mode_t mode) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (mkdirat, int, (int fd, char const *file, mode_t mode)); _GL_CXXALIASWARN (mkdirat); #elif defined GNULIB_POSIXCHECK # undef mkdirat # if HAVE_RAW_DECL_MKDIRAT _GL_WARN_ON_USE (mkdirat, "mkdirat is not portable - " "use gnulib module openat for portability"); # endif #endif #if @GNULIB_MKFIFO@ # if @REPLACE_MKFIFO@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mkfifo # define mkfifo rpl_mkfifo # endif _GL_FUNCDECL_RPL (mkfifo, int, (char const *file, mode_t mode) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mkfifo, int, (char const *file, mode_t mode)); # else # if !@HAVE_MKFIFO@ _GL_FUNCDECL_SYS (mkfifo, int, (char const *file, mode_t mode) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (mkfifo, int, (char const *file, mode_t mode)); # endif _GL_CXXALIASWARN (mkfifo); #elif defined GNULIB_POSIXCHECK # undef mkfifo # if HAVE_RAW_DECL_MKFIFO _GL_WARN_ON_USE (mkfifo, "mkfifo is not portable - " "use gnulib module mkfifo for portability"); # endif #endif #if @GNULIB_MKFIFOAT@ # if !@HAVE_MKFIFOAT@ _GL_FUNCDECL_SYS (mkfifoat, int, (int fd, char const *file, mode_t mode) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (mkfifoat, int, (int fd, char const *file, mode_t mode)); _GL_CXXALIASWARN (mkfifoat); #elif defined GNULIB_POSIXCHECK # undef mkfifoat # if HAVE_RAW_DECL_MKFIFOAT _GL_WARN_ON_USE (mkfifoat, "mkfifoat is not portable - " "use gnulib module mkfifoat for portability"); # endif #endif #if @GNULIB_MKNOD@ # if @REPLACE_MKNOD@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mknod # define mknod rpl_mknod # endif _GL_FUNCDECL_RPL (mknod, int, (char const *file, mode_t mode, dev_t dev) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mknod, int, (char const *file, mode_t mode, dev_t dev)); # else # if !@HAVE_MKNOD@ _GL_FUNCDECL_SYS (mknod, int, (char const *file, mode_t mode, dev_t dev) _GL_ARG_NONNULL ((1))); # endif /* Need to cast, because on OSF/1 5.1, the third parameter is '...'. */ _GL_CXXALIAS_SYS_CAST (mknod, int, (char const *file, mode_t mode, dev_t dev)); # endif _GL_CXXALIASWARN (mknod); #elif defined GNULIB_POSIXCHECK # undef mknod # if HAVE_RAW_DECL_MKNOD _GL_WARN_ON_USE (mknod, "mknod is not portable - " "use gnulib module mknod for portability"); # endif #endif #if @GNULIB_MKNODAT@ # if !@HAVE_MKNODAT@ _GL_FUNCDECL_SYS (mknodat, int, (int fd, char const *file, mode_t mode, dev_t dev) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (mknodat, int, (int fd, char const *file, mode_t mode, dev_t dev)); _GL_CXXALIASWARN (mknodat); #elif defined GNULIB_POSIXCHECK # undef mknodat # if HAVE_RAW_DECL_MKNODAT _GL_WARN_ON_USE (mknodat, "mknodat is not portable - " "use gnulib module mkfifoat for portability"); # endif #endif #if @GNULIB_STAT@ # if @REPLACE_STAT@ /* We can't use the object-like #define stat rpl_stat, because of struct stat. This means that rpl_stat will not be used if the user does (stat)(a,b). Oh well. */ # if defined _AIX && defined stat && defined _LARGE_FILES /* With _LARGE_FILES defined, AIX (only) defines stat to stat64, so we have to replace stat64() instead of stat(). */ # undef stat64 # define stat64(name, st) rpl_stat (name, st) # elif @WINDOWS_64_BIT_ST_SIZE@ /* Above, we define stat to _stati64. */ # if defined __MINGW32__ && defined _stati64 # ifndef _USE_32BIT_TIME_T /* The system headers define _stati64 to _stat64. */ # undef _stat64 # define _stat64(name, st) rpl_stat (name, st) # endif # elif defined _MSC_VER && defined _stati64 # ifdef _USE_32BIT_TIME_T /* The system headers define _stati64 to _stat32i64. */ # undef _stat32i64 # define _stat32i64(name, st) rpl_stat (name, st) # else /* The system headers define _stati64 to _stat64. */ # undef _stat64 # define _stat64(name, st) rpl_stat (name, st) # endif # else # undef _stati64 # define _stati64(name, st) rpl_stat (name, st) # endif # elif defined __MINGW32__ && defined stat # ifdef _USE_32BIT_TIME_T /* The system headers define stat to _stat32i64. */ # undef _stat32i64 # define _stat32i64(name, st) rpl_stat (name, st) # else /* The system headers define stat to _stat64. */ # undef _stat64 # define _stat64(name, st) rpl_stat (name, st) # endif # elif defined _MSC_VER && defined stat # ifdef _USE_32BIT_TIME_T /* The system headers define stat to _stat32. */ # undef _stat32 # define _stat32(name, st) rpl_stat (name, st) # else /* The system headers define stat to _stat64i32. */ # undef _stat64i32 # define _stat64i32(name, st) rpl_stat (name, st) # endif # else /* !(_AIX ||__MINGW32__ || _MSC_VER) */ # undef stat # define stat(name, st) rpl_stat (name, st) # endif /* !_LARGE_FILES */ _GL_EXTERN_C int stat (const char *name, struct stat *buf) _GL_ARG_NONNULL ((1, 2)); # endif #elif defined GNULIB_POSIXCHECK # undef stat # if HAVE_RAW_DECL_STAT _GL_WARN_ON_USE (stat, "stat is unportable - " "use gnulib module stat for portability"); # endif #endif #if @GNULIB_UTIMENSAT@ /* Use the rpl_ prefix also on Solaris <= 9, because on Solaris 9 our utimensat implementation relies on futimesat, which on Solaris 10 makes an invocation to utimensat that is meant to invoke the libc's utimensat(), not gnulib's utimensat(). */ # if @REPLACE_UTIMENSAT@ || (!@HAVE_UTIMENSAT@ && defined __sun) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef utimensat # define utimensat rpl_utimensat # endif _GL_FUNCDECL_RPL (utimensat, int, (int fd, char const *name, struct timespec const times[2], int flag) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (utimensat, int, (int fd, char const *name, struct timespec const times[2], int flag)); # else # if !@HAVE_UTIMENSAT@ _GL_FUNCDECL_SYS (utimensat, int, (int fd, char const *name, struct timespec const times[2], int flag) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (utimensat, int, (int fd, char const *name, struct timespec const times[2], int flag)); # endif # if @HAVE_UTIMENSAT@ _GL_CXXALIASWARN (utimensat); # endif #elif defined GNULIB_POSIXCHECK # undef utimensat # if HAVE_RAW_DECL_UTIMENSAT _GL_WARN_ON_USE (utimensat, "utimensat is not portable - " "use gnulib module utimensat for portability"); # endif #endif #endif /* _@GUARD_PREFIX@_SYS_STAT_H */ #endif /* _@GUARD_PREFIX@_SYS_STAT_H */ #endif gnuastro-0.2.33-8a3b/bootstrapped/tests/test-symlink.h0000644000175000017500000000607013004436755017613 00000000000000/* Tests of symlink. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ /* This file is designed to test both symlink(a,b) and symlinkat(a,AT_FDCWD,b). FUNC is the function to test. Assumes that BASE and ASSERT are already defined, and that appropriate headers are already included. If PRINT, warn before skipping symlink tests with status 77. */ static int test_symlink (int (*func) (char const *, char const *), bool print) { if (func ("nowhere", BASE "link1")) { if (print) fputs ("skipping test: symlinks not supported on this file system\n", stderr); return 77; } /* Some systems allow the creation of 0-length symlinks as a synonym for "."; but most reject it. */ { int status; errno = 0; status = func ("", BASE "link2"); if (status == -1) ASSERT (errno == ENOENT || errno == EINVAL); else { ASSERT (status == 0); ASSERT (unlink (BASE "link2") == 0); } } /* Sanity checks of failures. */ errno = 0; ASSERT (func ("nowhere", "") == -1); ASSERT (errno == ENOENT); errno = 0; ASSERT (func ("nowhere", ".") == -1); ASSERT (errno == EEXIST || errno == EINVAL); errno = 0; ASSERT (func ("somewhere", BASE "link1") == -1); ASSERT (errno == EEXIST); errno = 0; ASSERT (func ("nowhere", BASE "link2/") == -1); ASSERT (errno == ENOTDIR || errno == ENOENT); ASSERT (mkdir (BASE "dir", 0700) == 0); errno = 0; ASSERT (func ("nowhere", BASE "dir") == -1); ASSERT (errno == EEXIST); errno = 0; ASSERT (func ("nowhere", BASE "dir/") == -1); ASSERT (errno == EEXIST || errno == EINVAL); ASSERT (close (creat (BASE "file", 0600)) == 0); errno = 0; ASSERT (func ("nowhere", BASE "file") == -1); ASSERT (errno == EEXIST); errno = 0; ASSERT (func ("nowhere", BASE "file/") == -1); ASSERT (errno == EEXIST || errno == ENOTDIR || errno == ENOENT); /* Trailing slash must always be rejected. */ ASSERT (unlink (BASE "link1") == 0); ASSERT (func (BASE "link2", BASE "link1") == 0); errno = 0; ASSERT (func (BASE "nowhere", BASE "link1/") == -1); ASSERT (errno == EEXIST || errno == ENOTDIR || errno == ENOENT); errno = 0; ASSERT (unlink (BASE "link2") == -1); ASSERT (errno == ENOENT); /* Cleanup. */ ASSERT (rmdir (BASE "dir") == 0); ASSERT (unlink (BASE "file") == 0); ASSERT (unlink (BASE "link1") == 0); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-sys_wait.h0000644000175000017500000000361513004436755017771 00000000000000/* Test of macros shared between and . Copyright (C) 2010-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2010. */ static int test_sys_wait_macros (void) { /* Check subset of macros that must be visible here. Note that some of these macros are only portable when operating on an lvalue. */ int i; for (i = 0; i < 0x8000; i = (i ? i << 1 : 1)) { /* POSIX requires that for all valid process statuses, that exactly one of these three macros is true. But not all possible 16-bit values map to valid process status. Traditionally, 8 of the bits are for WIFEXITED, 7 of the bits to tell between WIFSIGNALED and WIFSTOPPED, and either 0x80 or 0x8000 to flag that core was also dumped. Since we don't know which byte is WIFEXITED, we skip the both possible bits that can signal core dump. */ if (i == 0x80) continue; if (!!WIFSIGNALED (i) + !!WIFEXITED (i) + !!WIFSTOPPED (i) != 1) return 1; } i = WEXITSTATUS (i) + WSTOPSIG (i) + WTERMSIG (i); switch (i) { #if 0 /* Gnulib doesn't guarantee these, yet. */ case WNOHANG: case WUNTRACED: #endif break; } return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-stat.h0000644000175000017500000000604213004436755017077 00000000000000/* Tests of stat. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ /* This file is designed to test both stat(n,buf) and fstatat(AT_FDCWD,n,buf,0). FUNC is the function to test. Assumes that BASE and ASSERT are already defined, and that appropriate headers are already included. If PRINT, warn before skipping symlink tests with status 77. */ static int test_stat_func (int (*func) (char const *, struct stat *), bool print) { struct stat st1; struct stat st2; char *cwd = getcwd (NULL, 0); ASSERT (cwd); ASSERT (func (".", &st1) == 0); ASSERT (func ("./", &st2) == 0); ASSERT (SAME_INODE (st1, st2)); ASSERT (func (cwd, &st2) == 0); ASSERT (SAME_INODE (st1, st2)); ASSERT (func ("/", &st1) == 0); ASSERT (func ("///", &st2) == 0); ASSERT (SAME_INODE (st1, st2)); errno = 0; ASSERT (func ("", &st1) == -1); ASSERT (errno == ENOENT); errno = 0; ASSERT (func ("nosuch", &st1) == -1); ASSERT (errno == ENOENT); errno = 0; ASSERT (func ("nosuch/", &st1) == -1); ASSERT (errno == ENOENT); ASSERT (close (creat (BASE "file", 0600)) == 0); ASSERT (func (BASE "file", &st1) == 0); errno = 0; ASSERT (func (BASE "file/", &st1) == -1); ASSERT (errno == ENOTDIR); /* Now for some symlink tests, where supported. We set up: link1 -> directory link2 -> file link3 -> dangling link4 -> loop then test behavior with trailing slash. */ if (symlink (".", BASE "link1") != 0) { ASSERT (unlink (BASE "file") == 0); if (print) fputs ("skipping test: symlinks not supported on this file system\n", stderr); return 77; } ASSERT (symlink (BASE "file", BASE "link2") == 0); ASSERT (symlink (BASE "nosuch", BASE "link3") == 0); ASSERT (symlink (BASE "link4", BASE "link4") == 0); ASSERT (func (BASE "link1/", &st1) == 0); ASSERT (S_ISDIR (st1.st_mode)); errno = 0; ASSERT (func (BASE "link2/", &st1) == -1); ASSERT (errno == ENOTDIR); errno = 0; ASSERT (func (BASE "link3/", &st1) == -1); ASSERT (errno == ENOENT); errno = 0; ASSERT (func (BASE "link4/", &st1) == -1); ASSERT (errno == ELOOP); /* Cleanup. */ ASSERT (unlink (BASE "file") == 0); ASSERT (unlink (BASE "link1") == 0); ASSERT (unlink (BASE "link2") == 0); ASSERT (unlink (BASE "link3") == 0); ASSERT (unlink (BASE "link4") == 0); free (cwd); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-setlocale2.sh0000755000175000017500000000134513004436755020350 00000000000000#!/bin/sh # Test locale names with likely unsupported encoding in Unix syntax. for name in ar_SA.ISO-8859-1 fr_FR.CP1251 zh_TW.GB18030 zh_CN.BIG5; do env LC_ALL=$name ./test-setlocale2${EXEEXT} 1 || exit 1 done # Test locale names with likely unsupported encoding in native Windows syntax. for name in "Arabic_Saudi Arabia.1252" "Arabic_Saudi Arabia.65001" \ French_France.65001 Japanese_Japan.65001 Turkish_Turkey.65001 \ Chinese_Taiwan.65001 Chinese_China.54936 Chinese_China.65001; do # Here we use 'env' to set the LC_ALL environment variable, because on # Solaris 11 2011-11, the /bin/sh refuses to do it for Turkish_Turkey.65001. env LC_ALL="$name" ./test-setlocale2${EXEEXT} 1 || exit 1 done exit 0 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-setlocale1.sh0000755000175000017500000000150613004436755020346 00000000000000#!/bin/sh : ${LOCALE_FR=fr_FR} : ${LOCALE_FR_UTF8=fr_FR.UTF-8} : ${LOCALE_JA=ja_JP} : ${LOCALE_ZH_CN=zh_CN.GB18030} if test $LOCALE_FR = none && test $LOCALE_FR_UTF8 = none \ && test $LOCALE_JA = none && test $LOCALE_ZH_CN = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no locale for testing is installed" else echo "Skipping test: no locale for testing is supported" fi exit 77 fi if test $LOCALE_FR != none; then LC_ALL=$LOCALE_FR ./test-setlocale1${EXEEXT} || exit 1 fi if test $LOCALE_FR_UTF8 != none; then LC_ALL=$LOCALE_FR_UTF8 ./test-setlocale1${EXEEXT} || exit 1 fi if test $LOCALE_JA != none; then LC_ALL=$LOCALE_JA ./test-setlocale1${EXEEXT} || exit 1 fi if test $LOCALE_ZH_CN != none; then LC_ALL=$LOCALE_ZH_CN ./test-setlocale1${EXEEXT} || exit 1 fi exit 0 gnuastro-0.2.33-8a3b/bootstrapped/tests/same-inode.h0000644000175000017500000000220213004436755017162 00000000000000/* Determine whether two stat buffers refer to the same file. Copyright (C) 2006, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef SAME_INODE_H # define SAME_INODE_H 1 # ifdef __VMS # define SAME_INODE(a, b) \ ((a).st_ino[0] == (b).st_ino[0] \ && (a).st_ino[1] == (b).st_ino[1] \ && (a).st_ino[2] == (b).st_ino[2] \ && (a).st_dev == (b).st_dev) # else # define SAME_INODE(a, b) \ ((a).st_ino == (b).st_ino \ && (a).st_dev == (b).st_dev) # endif #endif gnuastro-0.2.33-8a3b/bootstrapped/tests/pathmax.h0000644000175000017500000000555613004436755016622 00000000000000/* Define PATH_MAX somehow. Requires sys/types.h. Copyright (C) 1992, 1999, 2001, 2003, 2005, 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _PATHMAX_H # define _PATHMAX_H /* POSIX:2008 defines PATH_MAX to be the maximum number of bytes in a filename, including the terminating NUL byte. PATH_MAX is not defined on systems which have no limit on filename length, such as GNU/Hurd. This file does *not* define PATH_MAX always. Programs that use this file can handle the GNU/Hurd case in several ways: - Either with a package-wide handling, or with a per-file handling, - Either through a #ifdef PATH_MAX or through a fallback like #ifndef PATH_MAX # define PATH_MAX 8192 #endif or through a fallback like #ifndef PATH_MAX # define PATH_MAX pathconf ("/", _PC_PATH_MAX) #endif */ # include # include # ifndef _POSIX_PATH_MAX # define _POSIX_PATH_MAX 256 # endif /* Don't include sys/param.h if it already has been. */ # if defined HAVE_SYS_PARAM_H && !defined PATH_MAX && !defined MAXPATHLEN # include # endif # if !defined PATH_MAX && defined MAXPATHLEN # define PATH_MAX MAXPATHLEN # endif # ifdef __hpux /* On HP-UX, PATH_MAX designates the maximum number of bytes in a filename, *not* including the terminating NUL byte, and is set to 1023. Additionally, when _XOPEN_SOURCE is defined to 500 or more, PATH_MAX is not defined at all any more. */ # undef PATH_MAX # define PATH_MAX 1024 # endif # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* The page "Naming Files, Paths, and Namespaces" on msdn.microsoft.com, section "Maximum Path Length Limitation", explains that the maximum size of a filename, including the terminating NUL byte, is 260 = 3 + 256 + 1. This is the same value as - FILENAME_MAX in , - _MAX_PATH in , - MAX_PATH in . Undefine the original value, because mingw's gets it wrong. */ # undef PATH_MAX # define PATH_MAX 260 # endif #endif /* _PATHMAX_H */ gnuastro-0.2.33-8a3b/bootstrapped/tests/test-open.h0000644000175000017500000000646013004436755017071 00000000000000/* Test of opening a file descriptor. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ /* Make test_open always inline if we're using Fortify, which defines __always_inline to do that. Do nothing otherwise. This works around a glibc bug whereby 'open' cannot be used as a function pointer when _FORTIFY_SOURCE is positive. */ #if __GLIBC__ && defined __always_inline # define ALWAYS_INLINE __always_inline #else # define ALWAYS_INLINE #endif /* This file is designed to test both open(n,buf[,mode]) and openat(AT_FDCWD,n,buf[,mode]). FUNC is the function to test. Assumes that BASE and ASSERT are already defined, and that appropriate headers are already included. If PRINT, warn before skipping symlink tests with status 77. */ static ALWAYS_INLINE int test_open (int (*func) (char const *, int, ...), bool print) { int fd; /* Remove anything from prior partial run. */ unlink (BASE "file"); /* Cannot create directory. */ errno = 0; ASSERT (func ("nonexist.ent/", O_CREAT | O_RDONLY, 0600) == -1); ASSERT (errno == ENOTDIR || errno == EISDIR || errno == ENOENT || errno == EINVAL); /* Create a regular file. */ fd = func (BASE "file", O_CREAT | O_RDONLY, 0600); ASSERT (0 <= fd); ASSERT (close (fd) == 0); /* Trailing slash handling. */ errno = 0; ASSERT (func (BASE "file/", O_RDONLY) == -1); ASSERT (errno == ENOTDIR || errno == EISDIR || errno == EINVAL); /* Directories cannot be opened for writing. */ errno = 0; ASSERT (func (".", O_WRONLY) == -1); ASSERT (errno == EISDIR || errno == EACCES); /* /dev/null must exist, and be writable. */ fd = func ("/dev/null", O_RDONLY); ASSERT (0 <= fd); { char c; ASSERT (read (fd, &c, 1) == 0); } ASSERT (close (fd) == 0); fd = func ("/dev/null", O_WRONLY); ASSERT (0 <= fd); ASSERT (write (fd, "c", 1) == 1); ASSERT (close (fd) == 0); /* Although O_NONBLOCK on regular files can be ignored, it must not cause a failure. */ fd = func (BASE "file", O_NONBLOCK | O_RDONLY); ASSERT (0 <= fd); ASSERT (close (fd) == 0); /* Symlink handling, where supported. */ if (symlink (BASE "file", BASE "link") != 0) { ASSERT (unlink (BASE "file") == 0); if (print) fputs ("skipping test: symlinks not supported on this file system\n", stderr); return 77; } errno = 0; ASSERT (func (BASE "link/", O_RDONLY) == -1); ASSERT (errno == ENOTDIR); fd = func (BASE "link", O_RDONLY); ASSERT (0 <= fd); ASSERT (close (fd) == 0); /* Cleanup. */ ASSERT (unlink (BASE "file") == 0); ASSERT (unlink (BASE "link") == 0); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-nl_langinfo.sh0000755000175000017500000000066513004436755020605 00000000000000#!/bin/sh LC_ALL=C ./test-nl_langinfo${EXEEXT} 0 || exit 1 # Test whether a specific traditional locale is installed. : ${LOCALE_FR=fr_FR} if test $LOCALE_FR != none; then LC_ALL=$LOCALE_FR ./test-nl_langinfo${EXEEXT} 1 || exit 1 fi # Test whether a specific UTF-8 locale is installed. : ${LOCALE_FR_UTF8=fr_FR.UTF-8} if test $LOCALE_FR_UTF8 != none; then LC_ALL=$LOCALE_FR_UTF8 ./test-nl_langinfo${EXEEXT} 2 || exit 1 fi exit 0 gnuastro-0.2.33-8a3b/bootstrapped/tests/zerosize-ptr.h0000644000175000017500000000471613004436756017633 00000000000000/* Return a pointer to a zero-size object in memory. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* ISO C 99 does not allow memcmp(), memchr() etc. to be invoked with a NULL argument. Therefore this file produces a non-NULL pointer which cannot be dereferenced, if possible. */ #include /* Test whether mmap() and mprotect() are available. We don't use HAVE_MMAP, because AC_FUNC_MMAP would not define it on HP-UX. HAVE_MPROTECT is not enough, because mingw does not have mmap() but has an mprotect() function in libgcc.a. */ #if HAVE_SYS_MMAN_H && HAVE_MPROTECT # include # include # include # include /* Define MAP_FILE when it isn't otherwise. */ # ifndef MAP_FILE # define MAP_FILE 0 # endif #endif /* Return a pointer to a zero-size object in memory (that is, actually, a pointer to a page boundary where the previous page is readable and writable and the next page is neither readable not writable), if possible. Return NULL otherwise. */ static void * zerosize_ptr (void) { /* Use mmap and mprotect when they exist. Don't test HAVE_MMAP, because it is not defined on HP-UX 11 (since it does not support MAP_FIXED). */ #if HAVE_SYS_MMAN_H && HAVE_MPROTECT # if HAVE_MAP_ANONYMOUS const int flags = MAP_ANONYMOUS | MAP_PRIVATE; const int fd = -1; # else /* !HAVE_MAP_ANONYMOUS */ const int flags = MAP_FILE | MAP_PRIVATE; int fd = open ("/dev/zero", O_RDONLY, 0666); if (fd >= 0) # endif { int pagesize = getpagesize (); char *two_pages = (char *) mmap (NULL, 2 * pagesize, PROT_READ | PROT_WRITE, flags, fd, 0); if (two_pages != (char *)(-1) && mprotect (two_pages + pagesize, pagesize, PROT_NONE) == 0) return two_pages + pagesize; } #endif return NULL; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-mbsinit.sh0000755000175000017500000000056613004436755017764 00000000000000#!/bin/sh # Test whether a specific UTF-8 locale is installed. : ${LOCALE_FR_UTF8=fr_FR.UTF-8} if test $LOCALE_FR_UTF8 = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no french Unicode locale is installed" else echo "Skipping test: no french Unicode locale is supported" fi exit 77 fi LC_ALL=$LOCALE_FR_UTF8 \ ./test-mbsinit${EXEEXT} gnuastro-0.2.33-8a3b/bootstrapped/tests/test-mbrtowc-w32-5.sh0000755000175000017500000000012013004436755020531 00000000000000#!/bin/sh # Test a CP936 locale. ./test-mbrtowc-w32${EXEEXT} Chinese_China 936 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-mbrtowc-w32-4.sh0000755000175000017500000000012113004436755020531 00000000000000#!/bin/sh # Test a CP950 locale. ./test-mbrtowc-w32${EXEEXT} Chinese_Taiwan 950 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-mbrtowc-w32-3.sh0000755000175000017500000000012113004436755020530 00000000000000#!/bin/sh # Test a CP932 locale. ./test-mbrtowc-w32${EXEEXT} Japanese_Japan 932 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-mbrtowc-w32-2.sh0000755000175000017500000000013213004436755020531 00000000000000#!/bin/sh # Test a CP1256 locale. ./test-mbrtowc-w32${EXEEXT} "Arabic_Saudi Arabia" 1256 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-mbrtowc-w32-1.sh0000755000175000017500000000012213004436755020527 00000000000000#!/bin/sh # Test a CP1252 locale. ./test-mbrtowc-w32${EXEEXT} French_France 1252 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-mbrtowc5.sh0000755000175000017500000000022513004436755020051 00000000000000#!/bin/sh # Test whether the POSIX locale has encoding errors. LC_ALL=C \ ./test-mbrtowc${EXEEXT} 5 || exit LC_ALL=POSIX \ ./test-mbrtowc${EXEEXT} 5 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-mbrtowc4.sh0000755000175000017500000000060213004436755020047 00000000000000#!/bin/sh # Test whether a specific GB18030 locale is installed. : ${LOCALE_ZH_CN=zh_CN.GB18030} if test $LOCALE_ZH_CN = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no transitional chinese locale is installed" else echo "Skipping test: no transitional chinese locale is supported" fi exit 77 fi LC_ALL=$LOCALE_ZH_CN \ ./test-mbrtowc${EXEEXT} 4 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-mbrtowc3.sh0000755000175000017500000000056013004436755020051 00000000000000#!/bin/sh # Test whether a specific EUC-JP locale is installed. : ${LOCALE_JA=ja_JP} if test $LOCALE_JA = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no traditional japanese locale is installed" else echo "Skipping test: no traditional japanese locale is supported" fi exit 77 fi LC_ALL=$LOCALE_JA \ ./test-mbrtowc${EXEEXT} 3 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-mbrtowc2.sh0000755000175000017500000000057013004436755020051 00000000000000#!/bin/sh # Test whether a specific UTF-8 locale is installed. : ${LOCALE_FR_UTF8=fr_FR.UTF-8} if test $LOCALE_FR_UTF8 = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no french Unicode locale is installed" else echo "Skipping test: no french Unicode locale is supported" fi exit 77 fi LC_ALL=$LOCALE_FR_UTF8 \ ./test-mbrtowc${EXEEXT} 2 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-mbrtowc1.sh0000755000175000017500000000054513004436755020052 00000000000000#!/bin/sh # Test in an ISO-8859-1 or ISO-8859-15 locale. : ${LOCALE_FR=fr_FR} if test $LOCALE_FR = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no traditional french locale is installed" else echo "Skipping test: no traditional french locale is supported" fi exit 77 fi LC_ALL=$LOCALE_FR \ ./test-mbrtowc${EXEEXT} 1 gnuastro-0.2.33-8a3b/bootstrapped/tests/malloca.valgrind0000644000175000017500000000025713004436755020140 00000000000000# Suppress a valgrind message about use of uninitialized memory in freea(). # This use is OK because it provides only a speedup. { freea Memcheck:Cond fun:freea } gnuastro-0.2.33-8a3b/bootstrapped/tests/malloca.h0000644000175000017500000001107313004436755016557 00000000000000/* Safe automatic memory allocation. Copyright (C) 2003-2007, 2009-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2003. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _MALLOCA_H #define _MALLOCA_H #include #include #include #ifdef __cplusplus extern "C" { #endif /* safe_alloca(N) is equivalent to alloca(N) when it is safe to call alloca(N); otherwise it returns NULL. It either returns N bytes of memory allocated on the stack, that lasts until the function returns, or NULL. Use of safe_alloca should be avoided: - inside arguments of function calls - undefined behaviour, - in inline functions - the allocation may actually last until the calling function returns. */ #if HAVE_ALLOCA /* The OS usually guarantees only one guard page at the bottom of the stack, and a page size can be as small as 4096 bytes. So we cannot safely allocate anything larger than 4096 bytes. Also care for the possibility of a few compiler-allocated temporary stack slots. This must be a macro, not a function. */ # define safe_alloca(N) ((N) < 4032 ? alloca (N) : NULL) #else # define safe_alloca(N) ((void) (N), NULL) #endif /* malloca(N) is a safe variant of alloca(N). It allocates N bytes of memory allocated on the stack, that must be freed using freea() before the function returns. Upon failure, it returns NULL. */ #if HAVE_ALLOCA # define malloca(N) \ ((N) < 4032 - sa_increment \ ? (void *) ((char *) alloca ((N) + sa_increment) + sa_increment) \ : mmalloca (N)) #else # define malloca(N) \ mmalloca (N) #endif extern void * mmalloca (size_t n); /* Free a block of memory allocated through malloca(). */ #if HAVE_ALLOCA extern void freea (void *p); #else # define freea free #endif /* nmalloca(N,S) is an overflow-safe variant of malloca (N * S). It allocates an array of N objects, each with S bytes of memory, on the stack. S must be positive and N must be nonnegative. The array must be freed using freea() before the function returns. */ #if 1 /* Cf. the definition of xalloc_oversized. */ # define nmalloca(n, s) \ ((n) > (size_t) (sizeof (ptrdiff_t) <= sizeof (size_t) ? -1 : -2) / (s) \ ? NULL \ : malloca ((n) * (s))) #else extern void * nmalloca (size_t n, size_t s); #endif #ifdef __cplusplus } #endif /* ------------------- Auxiliary, non-public definitions ------------------- */ /* Determine the alignment of a type at compile time. */ #if defined __GNUC__ || defined __IBM__ALIGNOF__ # define sa_alignof __alignof__ #elif defined __cplusplus template struct sa_alignof_helper { char __slot1; type __slot2; }; # define sa_alignof(type) offsetof (sa_alignof_helper, __slot2) #elif defined __hpux /* Work around a HP-UX 10.20 cc bug with enums constants defined as offsetof values. */ # define sa_alignof(type) (sizeof (type) <= 4 ? 4 : 8) #elif defined _AIX /* Work around an AIX 3.2.5 xlc bug with enums constants defined as offsetof values. */ # define sa_alignof(type) (sizeof (type) <= 4 ? 4 : 8) #else # define sa_alignof(type) offsetof (struct { char __slot1; type __slot2; }, __slot2) #endif enum { /* The desired alignment of memory allocations is the maximum alignment among all elementary types. */ sa_alignment_long = sa_alignof (long), sa_alignment_double = sa_alignof (double), #if HAVE_LONG_LONG_INT sa_alignment_longlong = sa_alignof (long long), #endif sa_alignment_longdouble = sa_alignof (long double), sa_alignment_max = ((sa_alignment_long - 1) | (sa_alignment_double - 1) #if HAVE_LONG_LONG_INT | (sa_alignment_longlong - 1) #endif | (sa_alignment_longdouble - 1) ) + 1, /* The increment that guarantees room for a magic word must be >= sizeof (int) and a multiple of sa_alignment_max. */ sa_increment = ((sizeof (int) + sa_alignment_max - 1) / sa_alignment_max) * sa_alignment_max }; #endif /* _MALLOCA_H */ gnuastro-0.2.33-8a3b/bootstrapped/tests/test-lstat.h0000644000175000017500000000727013004436755017257 00000000000000/* Test of lstat() function. Copyright (C) 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Simon Josefsson, 2008; and Eric Blake, 2009. */ /* This file is designed to test both lstat(n,buf) and fstatat(AT_FDCWD,n,buf,AT_SYMLINK_NOFOLLOW). FUNC is the function to test. Assumes that BASE and ASSERT are already defined, and that appropriate headers are already included. If PRINT, warn before skipping symlink tests with status 77. */ static int test_lstat_func (int (*func) (char const *, struct stat *), bool print) { struct stat st1; struct stat st2; /* Test for common directories. */ ASSERT (func (".", &st1) == 0); ASSERT (func ("./", &st2) == 0); ASSERT (SAME_INODE (st1, st2)); ASSERT (S_ISDIR (st1.st_mode)); ASSERT (S_ISDIR (st2.st_mode)); ASSERT (func ("/", &st1) == 0); ASSERT (func ("///", &st2) == 0); ASSERT (SAME_INODE (st1, st2)); ASSERT (S_ISDIR (st1.st_mode)); ASSERT (S_ISDIR (st2.st_mode)); ASSERT (func ("..", &st1) == 0); ASSERT (S_ISDIR (st1.st_mode)); /* Test for error conditions. */ errno = 0; ASSERT (func ("", &st1) == -1); ASSERT (errno == ENOENT); errno = 0; ASSERT (func ("nosuch", &st1) == -1); ASSERT (errno == ENOENT); errno = 0; ASSERT (func ("nosuch/", &st1) == -1); ASSERT (errno == ENOENT); ASSERT (close (creat (BASE "file", 0600)) == 0); ASSERT (func (BASE "file", &st1) == 0); ASSERT (S_ISREG (st1.st_mode)); errno = 0; ASSERT (func (BASE "file/", &st1) == -1); ASSERT (errno == ENOTDIR); /* Now for some symlink tests, where supported. We set up: link1 -> directory link2 -> file link3 -> dangling link4 -> loop then test behavior both with and without trailing slash. */ if (symlink (".", BASE "link1") != 0) { ASSERT (unlink (BASE "file") == 0); if (print) fputs ("skipping test: symlinks not supported on this file system\n", stderr); return 77; } ASSERT (symlink (BASE "file", BASE "link2") == 0); ASSERT (symlink (BASE "nosuch", BASE "link3") == 0); ASSERT (symlink (BASE "link4", BASE "link4") == 0); ASSERT (func (BASE "link1", &st1) == 0); ASSERT (S_ISLNK (st1.st_mode)); ASSERT (func (BASE "link1/", &st1) == 0); ASSERT (stat (BASE "link1", &st2) == 0); ASSERT (S_ISDIR (st1.st_mode)); ASSERT (S_ISDIR (st2.st_mode)); ASSERT (SAME_INODE (st1, st2)); ASSERT (func (BASE "link2", &st1) == 0); ASSERT (S_ISLNK (st1.st_mode)); errno = 0; ASSERT (func (BASE "link2/", &st1) == -1); ASSERT (errno == ENOTDIR); ASSERT (func (BASE "link3", &st1) == 0); ASSERT (S_ISLNK (st1.st_mode)); errno = 0; ASSERT (func (BASE "link3/", &st1) == -1); ASSERT (errno == ENOENT); ASSERT (func (BASE "link4", &st1) == 0); ASSERT (S_ISLNK (st1.st_mode)); errno = 0; ASSERT (func (BASE "link4/", &st1) == -1); ASSERT (errno == ELOOP); /* Cleanup. */ ASSERT (unlink (BASE "file") == 0); ASSERT (unlink (BASE "link1") == 0); ASSERT (unlink (BASE "link2") == 0); ASSERT (unlink (BASE "link3") == 0); ASSERT (unlink (BASE "link4") == 0); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/localename.h0000644000175000017500000001102713004436755017246 00000000000000/* Determine name of the currently selected locale. Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _GL_LOCALENAME_H #define _GL_LOCALENAME_H #ifdef __cplusplus extern "C" { #endif /* Determine the current locale's name. It considers both the POSIX notion of locale name (see functions gl_locale_name_thread and gl_locale_name_posix) and the system notion of locale name (see function gl_locale_name_default). CATEGORY is a locale category abbreviation, as defined in , but not LC_ALL. E.g. LC_MESSAGES. CATEGORYNAME is the name of CATEGORY as a string, e.g. "LC_MESSAGES". Return the locale category's name, canonicalized into XPG syntax language[_territory][.codeset][@modifier] The codeset part in the result is not reliable; the locale_charset() should be used for codeset information instead. The result must not be freed; it is statically allocated. */ extern const char * gl_locale_name (int category, const char *categoryname); /* Determine the current per-thread locale's name, as specified by uselocale() calls. CATEGORY is a locale category abbreviation, as defined in , but not LC_ALL. E.g. LC_MESSAGES. CATEGORYNAME is the name of CATEGORY as a string, e.g. "LC_MESSAGES". Return the locale category's name, canonicalized into XPG syntax language[_territory][.codeset][@modifier] or NULL if no locale has been specified for the current thread. The codeset part in the result is not reliable; the locale_charset() should be used for codeset information instead. The result must not be freed; it is statically allocated. */ extern const char * gl_locale_name_thread (int category, const char *categoryname); /* Determine the thread-independent current locale's name, as specified by setlocale() calls or by environment variables. CATEGORY is a locale category abbreviation, as defined in , but not LC_ALL. E.g. LC_MESSAGES. CATEGORYNAME is the name of CATEGORY as a string, e.g. "LC_MESSAGES". Return the locale category's name, canonicalized into XPG syntax language[_territory][.codeset][@modifier] or NULL if no locale has been specified to setlocale() or by environment variables. The codeset part in the result is not reliable; the locale_charset() should be used for codeset information instead. The result must not be freed; it is statically allocated. */ extern const char * gl_locale_name_posix (int category, const char *categoryname); /* Determine the default locale's name, as specified by environment variables. Return the locale category's name, or NULL if no locale has been specified by environment variables. The result must not be freed; it is statically allocated. */ extern const char * gl_locale_name_environ (int category, const char *categoryname); /* Determine the default locale's name. This is the current locale's name, if not specified by uselocale() calls, by setlocale() calls, or by environment variables. This locale name is usually determined by systems settings that the user can manipulate through a GUI. Quoting POSIX:2001: "All implementations shall define a locale as the default locale, to be invoked when no environment variables are set, or set to the empty string. This default locale can be the C locale or any other implementation-defined locale. Some implementations may provide facilities for local installation administrators to set the default locale, customizing it for each location. IEEE Std 1003.1-2001 does not require such a facility." The result must not be freed; it is statically allocated. */ extern const char * gl_locale_name_default (void) #if !(HAVE_CFLOCALECOPYCURRENT || HAVE_CFPREFERENCESCOPYAPPVALUE \ || defined _WIN32 || defined __WIN32__ || defined __CYGWIN__) _GL_ATTRIBUTE_CONST #endif ; #ifdef __cplusplus } #endif #endif /* _GL_LOCALENAME_H */ gnuastro-0.2.33-8a3b/bootstrapped/tests/inttypes.in.h0000644000175000017500000006476113004436755017447 00000000000000/* Copyright (C) 2006-2016 Free Software Foundation, Inc. Written by Paul Eggert, Bruno Haible, Derek Price. This file is part of gnulib. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* * ISO C 99 for platforms that lack it. * */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* Include the original if it exists, and if this file has not been included yet or if this file includes gnulib stdint.h which in turn includes this file. The include_next requires a split double-inclusion guard. */ #if ! defined INTTYPES_H || defined _GL_JUST_INCLUDE_SYSTEM_INTTYPES_H # if @HAVE_INTTYPES_H@ /* Some pre-C++11 implementations need this. */ # if defined __cplusplus && ! defined __STDC_FORMAT_MACROS # define __STDC_FORMAT_MACROS 1 # endif # @INCLUDE_NEXT@ @NEXT_INTTYPES_H@ # endif #endif #if ! defined INTTYPES_H && ! defined _GL_JUST_INCLUDE_SYSTEM_INTTYPES_H #define INTTYPES_H /* Include or the gnulib replacement. But avoid namespace pollution on glibc systems. */ #ifndef __GLIBC__ # include #endif /* Get CHAR_BIT. */ #include /* On mingw, __USE_MINGW_ANSI_STDIO only works if is also included */ #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # include #endif #if !(INT_MIN == INT32_MIN && INT_MAX == INT32_MAX) # error "This file assumes that 'int' has exactly 32 bits. Please report your platform and compiler to ." #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* 7.8.1 Macros for format specifiers */ #if defined _TNS_R_TARGET /* Tandem NonStop R series and compatible platforms released before July 2005 support %Ld but not %lld. */ # define _LONG_LONG_FORMAT_PREFIX "L" #else # define _LONG_LONG_FORMAT_PREFIX "ll" #endif #if !defined PRId8 || @PRI_MACROS_BROKEN@ # undef PRId8 # ifdef INT8_MAX # define PRId8 "d" # endif #endif #if !defined PRIi8 || @PRI_MACROS_BROKEN@ # undef PRIi8 # ifdef INT8_MAX # define PRIi8 "i" # endif #endif #if !defined PRIo8 || @PRI_MACROS_BROKEN@ # undef PRIo8 # ifdef UINT8_MAX # define PRIo8 "o" # endif #endif #if !defined PRIu8 || @PRI_MACROS_BROKEN@ # undef PRIu8 # ifdef UINT8_MAX # define PRIu8 "u" # endif #endif #if !defined PRIx8 || @PRI_MACROS_BROKEN@ # undef PRIx8 # ifdef UINT8_MAX # define PRIx8 "x" # endif #endif #if !defined PRIX8 || @PRI_MACROS_BROKEN@ # undef PRIX8 # ifdef UINT8_MAX # define PRIX8 "X" # endif #endif #if !defined PRId16 || @PRI_MACROS_BROKEN@ # undef PRId16 # ifdef INT16_MAX # define PRId16 "d" # endif #endif #if !defined PRIi16 || @PRI_MACROS_BROKEN@ # undef PRIi16 # ifdef INT16_MAX # define PRIi16 "i" # endif #endif #if !defined PRIo16 || @PRI_MACROS_BROKEN@ # undef PRIo16 # ifdef UINT16_MAX # define PRIo16 "o" # endif #endif #if !defined PRIu16 || @PRI_MACROS_BROKEN@ # undef PRIu16 # ifdef UINT16_MAX # define PRIu16 "u" # endif #endif #if !defined PRIx16 || @PRI_MACROS_BROKEN@ # undef PRIx16 # ifdef UINT16_MAX # define PRIx16 "x" # endif #endif #if !defined PRIX16 || @PRI_MACROS_BROKEN@ # undef PRIX16 # ifdef UINT16_MAX # define PRIX16 "X" # endif #endif #if !defined PRId32 || @PRI_MACROS_BROKEN@ # undef PRId32 # ifdef INT32_MAX # define PRId32 "d" # endif #endif #if !defined PRIi32 || @PRI_MACROS_BROKEN@ # undef PRIi32 # ifdef INT32_MAX # define PRIi32 "i" # endif #endif #if !defined PRIo32 || @PRI_MACROS_BROKEN@ # undef PRIo32 # ifdef UINT32_MAX # define PRIo32 "o" # endif #endif #if !defined PRIu32 || @PRI_MACROS_BROKEN@ # undef PRIu32 # ifdef UINT32_MAX # define PRIu32 "u" # endif #endif #if !defined PRIx32 || @PRI_MACROS_BROKEN@ # undef PRIx32 # ifdef UINT32_MAX # define PRIx32 "x" # endif #endif #if !defined PRIX32 || @PRI_MACROS_BROKEN@ # undef PRIX32 # ifdef UINT32_MAX # define PRIX32 "X" # endif #endif #ifdef INT64_MAX # if (@APPLE_UNIVERSAL_BUILD@ ? defined _LP64 : @INT64_MAX_EQ_LONG_MAX@) # define _PRI64_PREFIX "l" # elif defined _MSC_VER || defined __MINGW32__ # define _PRI64_PREFIX "I64" # elif @HAVE_LONG_LONG_INT@ && LONG_MAX >> 30 == 1 # define _PRI64_PREFIX _LONG_LONG_FORMAT_PREFIX # endif # if !defined PRId64 || @PRI_MACROS_BROKEN@ # undef PRId64 # define PRId64 _PRI64_PREFIX "d" # endif # if !defined PRIi64 || @PRI_MACROS_BROKEN@ # undef PRIi64 # define PRIi64 _PRI64_PREFIX "i" # endif #endif #ifdef UINT64_MAX # if (@APPLE_UNIVERSAL_BUILD@ ? defined _LP64 : @UINT64_MAX_EQ_ULONG_MAX@) # define _PRIu64_PREFIX "l" # elif defined _MSC_VER || defined __MINGW32__ # define _PRIu64_PREFIX "I64" # elif @HAVE_UNSIGNED_LONG_LONG_INT@ && ULONG_MAX >> 31 == 1 # define _PRIu64_PREFIX _LONG_LONG_FORMAT_PREFIX # endif # if !defined PRIo64 || @PRI_MACROS_BROKEN@ # undef PRIo64 # define PRIo64 _PRIu64_PREFIX "o" # endif # if !defined PRIu64 || @PRI_MACROS_BROKEN@ # undef PRIu64 # define PRIu64 _PRIu64_PREFIX "u" # endif # if !defined PRIx64 || @PRI_MACROS_BROKEN@ # undef PRIx64 # define PRIx64 _PRIu64_PREFIX "x" # endif # if !defined PRIX64 || @PRI_MACROS_BROKEN@ # undef PRIX64 # define PRIX64 _PRIu64_PREFIX "X" # endif #endif #if !defined PRIdLEAST8 || @PRI_MACROS_BROKEN@ # undef PRIdLEAST8 # define PRIdLEAST8 "d" #endif #if !defined PRIiLEAST8 || @PRI_MACROS_BROKEN@ # undef PRIiLEAST8 # define PRIiLEAST8 "i" #endif #if !defined PRIoLEAST8 || @PRI_MACROS_BROKEN@ # undef PRIoLEAST8 # define PRIoLEAST8 "o" #endif #if !defined PRIuLEAST8 || @PRI_MACROS_BROKEN@ # undef PRIuLEAST8 # define PRIuLEAST8 "u" #endif #if !defined PRIxLEAST8 || @PRI_MACROS_BROKEN@ # undef PRIxLEAST8 # define PRIxLEAST8 "x" #endif #if !defined PRIXLEAST8 || @PRI_MACROS_BROKEN@ # undef PRIXLEAST8 # define PRIXLEAST8 "X" #endif #if !defined PRIdLEAST16 || @PRI_MACROS_BROKEN@ # undef PRIdLEAST16 # define PRIdLEAST16 "d" #endif #if !defined PRIiLEAST16 || @PRI_MACROS_BROKEN@ # undef PRIiLEAST16 # define PRIiLEAST16 "i" #endif #if !defined PRIoLEAST16 || @PRI_MACROS_BROKEN@ # undef PRIoLEAST16 # define PRIoLEAST16 "o" #endif #if !defined PRIuLEAST16 || @PRI_MACROS_BROKEN@ # undef PRIuLEAST16 # define PRIuLEAST16 "u" #endif #if !defined PRIxLEAST16 || @PRI_MACROS_BROKEN@ # undef PRIxLEAST16 # define PRIxLEAST16 "x" #endif #if !defined PRIXLEAST16 || @PRI_MACROS_BROKEN@ # undef PRIXLEAST16 # define PRIXLEAST16 "X" #endif #if !defined PRIdLEAST32 || @PRI_MACROS_BROKEN@ # undef PRIdLEAST32 # define PRIdLEAST32 "d" #endif #if !defined PRIiLEAST32 || @PRI_MACROS_BROKEN@ # undef PRIiLEAST32 # define PRIiLEAST32 "i" #endif #if !defined PRIoLEAST32 || @PRI_MACROS_BROKEN@ # undef PRIoLEAST32 # define PRIoLEAST32 "o" #endif #if !defined PRIuLEAST32 || @PRI_MACROS_BROKEN@ # undef PRIuLEAST32 # define PRIuLEAST32 "u" #endif #if !defined PRIxLEAST32 || @PRI_MACROS_BROKEN@ # undef PRIxLEAST32 # define PRIxLEAST32 "x" #endif #if !defined PRIXLEAST32 || @PRI_MACROS_BROKEN@ # undef PRIXLEAST32 # define PRIXLEAST32 "X" #endif #ifdef INT64_MAX # if !defined PRIdLEAST64 || @PRI_MACROS_BROKEN@ # undef PRIdLEAST64 # define PRIdLEAST64 PRId64 # endif # if !defined PRIiLEAST64 || @PRI_MACROS_BROKEN@ # undef PRIiLEAST64 # define PRIiLEAST64 PRIi64 # endif #endif #ifdef UINT64_MAX # if !defined PRIoLEAST64 || @PRI_MACROS_BROKEN@ # undef PRIoLEAST64 # define PRIoLEAST64 PRIo64 # endif # if !defined PRIuLEAST64 || @PRI_MACROS_BROKEN@ # undef PRIuLEAST64 # define PRIuLEAST64 PRIu64 # endif # if !defined PRIxLEAST64 || @PRI_MACROS_BROKEN@ # undef PRIxLEAST64 # define PRIxLEAST64 PRIx64 # endif # if !defined PRIXLEAST64 || @PRI_MACROS_BROKEN@ # undef PRIXLEAST64 # define PRIXLEAST64 PRIX64 # endif #endif #if !defined PRIdFAST8 || @PRI_MACROS_BROKEN@ # undef PRIdFAST8 # if INT_FAST8_MAX > INT32_MAX # define PRIdFAST8 PRId64 # else # define PRIdFAST8 "d" # endif #endif #if !defined PRIiFAST8 || @PRI_MACROS_BROKEN@ # undef PRIiFAST8 # if INT_FAST8_MAX > INT32_MAX # define PRIiFAST8 PRIi64 # else # define PRIiFAST8 "i" # endif #endif #if !defined PRIoFAST8 || @PRI_MACROS_BROKEN@ # undef PRIoFAST8 # if UINT_FAST8_MAX > UINT32_MAX # define PRIoFAST8 PRIo64 # else # define PRIoFAST8 "o" # endif #endif #if !defined PRIuFAST8 || @PRI_MACROS_BROKEN@ # undef PRIuFAST8 # if UINT_FAST8_MAX > UINT32_MAX # define PRIuFAST8 PRIu64 # else # define PRIuFAST8 "u" # endif #endif #if !defined PRIxFAST8 || @PRI_MACROS_BROKEN@ # undef PRIxFAST8 # if UINT_FAST8_MAX > UINT32_MAX # define PRIxFAST8 PRIx64 # else # define PRIxFAST8 "x" # endif #endif #if !defined PRIXFAST8 || @PRI_MACROS_BROKEN@ # undef PRIXFAST8 # if UINT_FAST8_MAX > UINT32_MAX # define PRIXFAST8 PRIX64 # else # define PRIXFAST8 "X" # endif #endif #if !defined PRIdFAST16 || @PRI_MACROS_BROKEN@ # undef PRIdFAST16 # if INT_FAST16_MAX > INT32_MAX # define PRIdFAST16 PRId64 # else # define PRIdFAST16 "d" # endif #endif #if !defined PRIiFAST16 || @PRI_MACROS_BROKEN@ # undef PRIiFAST16 # if INT_FAST16_MAX > INT32_MAX # define PRIiFAST16 PRIi64 # else # define PRIiFAST16 "i" # endif #endif #if !defined PRIoFAST16 || @PRI_MACROS_BROKEN@ # undef PRIoFAST16 # if UINT_FAST16_MAX > UINT32_MAX # define PRIoFAST16 PRIo64 # else # define PRIoFAST16 "o" # endif #endif #if !defined PRIuFAST16 || @PRI_MACROS_BROKEN@ # undef PRIuFAST16 # if UINT_FAST16_MAX > UINT32_MAX # define PRIuFAST16 PRIu64 # else # define PRIuFAST16 "u" # endif #endif #if !defined PRIxFAST16 || @PRI_MACROS_BROKEN@ # undef PRIxFAST16 # if UINT_FAST16_MAX > UINT32_MAX # define PRIxFAST16 PRIx64 # else # define PRIxFAST16 "x" # endif #endif #if !defined PRIXFAST16 || @PRI_MACROS_BROKEN@ # undef PRIXFAST16 # if UINT_FAST16_MAX > UINT32_MAX # define PRIXFAST16 PRIX64 # else # define PRIXFAST16 "X" # endif #endif #if !defined PRIdFAST32 || @PRI_MACROS_BROKEN@ # undef PRIdFAST32 # if INT_FAST32_MAX > INT32_MAX # define PRIdFAST32 PRId64 # else # define PRIdFAST32 "d" # endif #endif #if !defined PRIiFAST32 || @PRI_MACROS_BROKEN@ # undef PRIiFAST32 # if INT_FAST32_MAX > INT32_MAX # define PRIiFAST32 PRIi64 # else # define PRIiFAST32 "i" # endif #endif #if !defined PRIoFAST32 || @PRI_MACROS_BROKEN@ # undef PRIoFAST32 # if UINT_FAST32_MAX > UINT32_MAX # define PRIoFAST32 PRIo64 # else # define PRIoFAST32 "o" # endif #endif #if !defined PRIuFAST32 || @PRI_MACROS_BROKEN@ # undef PRIuFAST32 # if UINT_FAST32_MAX > UINT32_MAX # define PRIuFAST32 PRIu64 # else # define PRIuFAST32 "u" # endif #endif #if !defined PRIxFAST32 || @PRI_MACROS_BROKEN@ # undef PRIxFAST32 # if UINT_FAST32_MAX > UINT32_MAX # define PRIxFAST32 PRIx64 # else # define PRIxFAST32 "x" # endif #endif #if !defined PRIXFAST32 || @PRI_MACROS_BROKEN@ # undef PRIXFAST32 # if UINT_FAST32_MAX > UINT32_MAX # define PRIXFAST32 PRIX64 # else # define PRIXFAST32 "X" # endif #endif #ifdef INT64_MAX # if !defined PRIdFAST64 || @PRI_MACROS_BROKEN@ # undef PRIdFAST64 # define PRIdFAST64 PRId64 # endif # if !defined PRIiFAST64 || @PRI_MACROS_BROKEN@ # undef PRIiFAST64 # define PRIiFAST64 PRIi64 # endif #endif #ifdef UINT64_MAX # if !defined PRIoFAST64 || @PRI_MACROS_BROKEN@ # undef PRIoFAST64 # define PRIoFAST64 PRIo64 # endif # if !defined PRIuFAST64 || @PRI_MACROS_BROKEN@ # undef PRIuFAST64 # define PRIuFAST64 PRIu64 # endif # if !defined PRIxFAST64 || @PRI_MACROS_BROKEN@ # undef PRIxFAST64 # define PRIxFAST64 PRIx64 # endif # if !defined PRIXFAST64 || @PRI_MACROS_BROKEN@ # undef PRIXFAST64 # define PRIXFAST64 PRIX64 # endif #endif #if !defined PRIdMAX || @PRI_MACROS_BROKEN@ # undef PRIdMAX # if @INT32_MAX_LT_INTMAX_MAX@ # define PRIdMAX PRId64 # else # define PRIdMAX "ld" # endif #endif #if !defined PRIiMAX || @PRI_MACROS_BROKEN@ # undef PRIiMAX # if @INT32_MAX_LT_INTMAX_MAX@ # define PRIiMAX PRIi64 # else # define PRIiMAX "li" # endif #endif #if !defined PRIoMAX || @PRI_MACROS_BROKEN@ # undef PRIoMAX # if @UINT32_MAX_LT_UINTMAX_MAX@ # define PRIoMAX PRIo64 # else # define PRIoMAX "lo" # endif #endif #if !defined PRIuMAX || @PRI_MACROS_BROKEN@ # undef PRIuMAX # if @UINT32_MAX_LT_UINTMAX_MAX@ # define PRIuMAX PRIu64 # else # define PRIuMAX "lu" # endif #endif #if !defined PRIxMAX || @PRI_MACROS_BROKEN@ # undef PRIxMAX # if @UINT32_MAX_LT_UINTMAX_MAX@ # define PRIxMAX PRIx64 # else # define PRIxMAX "lx" # endif #endif #if !defined PRIXMAX || @PRI_MACROS_BROKEN@ # undef PRIXMAX # if @UINT32_MAX_LT_UINTMAX_MAX@ # define PRIXMAX PRIX64 # else # define PRIXMAX "lX" # endif #endif #if !defined PRIdPTR || @PRI_MACROS_BROKEN@ # undef PRIdPTR # ifdef INTPTR_MAX # define PRIdPTR @PRIPTR_PREFIX@ "d" # endif #endif #if !defined PRIiPTR || @PRI_MACROS_BROKEN@ # undef PRIiPTR # ifdef INTPTR_MAX # define PRIiPTR @PRIPTR_PREFIX@ "i" # endif #endif #if !defined PRIoPTR || @PRI_MACROS_BROKEN@ # undef PRIoPTR # ifdef UINTPTR_MAX # define PRIoPTR @PRIPTR_PREFIX@ "o" # endif #endif #if !defined PRIuPTR || @PRI_MACROS_BROKEN@ # undef PRIuPTR # ifdef UINTPTR_MAX # define PRIuPTR @PRIPTR_PREFIX@ "u" # endif #endif #if !defined PRIxPTR || @PRI_MACROS_BROKEN@ # undef PRIxPTR # ifdef UINTPTR_MAX # define PRIxPTR @PRIPTR_PREFIX@ "x" # endif #endif #if !defined PRIXPTR || @PRI_MACROS_BROKEN@ # undef PRIXPTR # ifdef UINTPTR_MAX # define PRIXPTR @PRIPTR_PREFIX@ "X" # endif #endif #if !defined SCNd8 || @PRI_MACROS_BROKEN@ # undef SCNd8 # ifdef INT8_MAX # define SCNd8 "hhd" # endif #endif #if !defined SCNi8 || @PRI_MACROS_BROKEN@ # undef SCNi8 # ifdef INT8_MAX # define SCNi8 "hhi" # endif #endif #if !defined SCNo8 || @PRI_MACROS_BROKEN@ # undef SCNo8 # ifdef UINT8_MAX # define SCNo8 "hho" # endif #endif #if !defined SCNu8 || @PRI_MACROS_BROKEN@ # undef SCNu8 # ifdef UINT8_MAX # define SCNu8 "hhu" # endif #endif #if !defined SCNx8 || @PRI_MACROS_BROKEN@ # undef SCNx8 # ifdef UINT8_MAX # define SCNx8 "hhx" # endif #endif #if !defined SCNd16 || @PRI_MACROS_BROKEN@ # undef SCNd16 # ifdef INT16_MAX # define SCNd16 "hd" # endif #endif #if !defined SCNi16 || @PRI_MACROS_BROKEN@ # undef SCNi16 # ifdef INT16_MAX # define SCNi16 "hi" # endif #endif #if !defined SCNo16 || @PRI_MACROS_BROKEN@ # undef SCNo16 # ifdef UINT16_MAX # define SCNo16 "ho" # endif #endif #if !defined SCNu16 || @PRI_MACROS_BROKEN@ # undef SCNu16 # ifdef UINT16_MAX # define SCNu16 "hu" # endif #endif #if !defined SCNx16 || @PRI_MACROS_BROKEN@ # undef SCNx16 # ifdef UINT16_MAX # define SCNx16 "hx" # endif #endif #if !defined SCNd32 || @PRI_MACROS_BROKEN@ # undef SCNd32 # ifdef INT32_MAX # define SCNd32 "d" # endif #endif #if !defined SCNi32 || @PRI_MACROS_BROKEN@ # undef SCNi32 # ifdef INT32_MAX # define SCNi32 "i" # endif #endif #if !defined SCNo32 || @PRI_MACROS_BROKEN@ # undef SCNo32 # ifdef UINT32_MAX # define SCNo32 "o" # endif #endif #if !defined SCNu32 || @PRI_MACROS_BROKEN@ # undef SCNu32 # ifdef UINT32_MAX # define SCNu32 "u" # endif #endif #if !defined SCNx32 || @PRI_MACROS_BROKEN@ # undef SCNx32 # ifdef UINT32_MAX # define SCNx32 "x" # endif #endif #ifdef INT64_MAX # if (@APPLE_UNIVERSAL_BUILD@ ? defined _LP64 : @INT64_MAX_EQ_LONG_MAX@) # define _SCN64_PREFIX "l" # elif defined _MSC_VER || defined __MINGW32__ # define _SCN64_PREFIX "I64" # elif @HAVE_LONG_LONG_INT@ && LONG_MAX >> 30 == 1 # define _SCN64_PREFIX _LONG_LONG_FORMAT_PREFIX # endif # if !defined SCNd64 || @PRI_MACROS_BROKEN@ # undef SCNd64 # define SCNd64 _SCN64_PREFIX "d" # endif # if !defined SCNi64 || @PRI_MACROS_BROKEN@ # undef SCNi64 # define SCNi64 _SCN64_PREFIX "i" # endif #endif #ifdef UINT64_MAX # if (@APPLE_UNIVERSAL_BUILD@ ? defined _LP64 : @UINT64_MAX_EQ_ULONG_MAX@) # define _SCNu64_PREFIX "l" # elif defined _MSC_VER || defined __MINGW32__ # define _SCNu64_PREFIX "I64" # elif @HAVE_UNSIGNED_LONG_LONG_INT@ && ULONG_MAX >> 31 == 1 # define _SCNu64_PREFIX _LONG_LONG_FORMAT_PREFIX # endif # if !defined SCNo64 || @PRI_MACROS_BROKEN@ # undef SCNo64 # define SCNo64 _SCNu64_PREFIX "o" # endif # if !defined SCNu64 || @PRI_MACROS_BROKEN@ # undef SCNu64 # define SCNu64 _SCNu64_PREFIX "u" # endif # if !defined SCNx64 || @PRI_MACROS_BROKEN@ # undef SCNx64 # define SCNx64 _SCNu64_PREFIX "x" # endif #endif #if !defined SCNdLEAST8 || @PRI_MACROS_BROKEN@ # undef SCNdLEAST8 # define SCNdLEAST8 "hhd" #endif #if !defined SCNiLEAST8 || @PRI_MACROS_BROKEN@ # undef SCNiLEAST8 # define SCNiLEAST8 "hhi" #endif #if !defined SCNoLEAST8 || @PRI_MACROS_BROKEN@ # undef SCNoLEAST8 # define SCNoLEAST8 "hho" #endif #if !defined SCNuLEAST8 || @PRI_MACROS_BROKEN@ # undef SCNuLEAST8 # define SCNuLEAST8 "hhu" #endif #if !defined SCNxLEAST8 || @PRI_MACROS_BROKEN@ # undef SCNxLEAST8 # define SCNxLEAST8 "hhx" #endif #if !defined SCNdLEAST16 || @PRI_MACROS_BROKEN@ # undef SCNdLEAST16 # define SCNdLEAST16 "hd" #endif #if !defined SCNiLEAST16 || @PRI_MACROS_BROKEN@ # undef SCNiLEAST16 # define SCNiLEAST16 "hi" #endif #if !defined SCNoLEAST16 || @PRI_MACROS_BROKEN@ # undef SCNoLEAST16 # define SCNoLEAST16 "ho" #endif #if !defined SCNuLEAST16 || @PRI_MACROS_BROKEN@ # undef SCNuLEAST16 # define SCNuLEAST16 "hu" #endif #if !defined SCNxLEAST16 || @PRI_MACROS_BROKEN@ # undef SCNxLEAST16 # define SCNxLEAST16 "hx" #endif #if !defined SCNdLEAST32 || @PRI_MACROS_BROKEN@ # undef SCNdLEAST32 # define SCNdLEAST32 "d" #endif #if !defined SCNiLEAST32 || @PRI_MACROS_BROKEN@ # undef SCNiLEAST32 # define SCNiLEAST32 "i" #endif #if !defined SCNoLEAST32 || @PRI_MACROS_BROKEN@ # undef SCNoLEAST32 # define SCNoLEAST32 "o" #endif #if !defined SCNuLEAST32 || @PRI_MACROS_BROKEN@ # undef SCNuLEAST32 # define SCNuLEAST32 "u" #endif #if !defined SCNxLEAST32 || @PRI_MACROS_BROKEN@ # undef SCNxLEAST32 # define SCNxLEAST32 "x" #endif #ifdef INT64_MAX # if !defined SCNdLEAST64 || @PRI_MACROS_BROKEN@ # undef SCNdLEAST64 # define SCNdLEAST64 SCNd64 # endif # if !defined SCNiLEAST64 || @PRI_MACROS_BROKEN@ # undef SCNiLEAST64 # define SCNiLEAST64 SCNi64 # endif #endif #ifdef UINT64_MAX # if !defined SCNoLEAST64 || @PRI_MACROS_BROKEN@ # undef SCNoLEAST64 # define SCNoLEAST64 SCNo64 # endif # if !defined SCNuLEAST64 || @PRI_MACROS_BROKEN@ # undef SCNuLEAST64 # define SCNuLEAST64 SCNu64 # endif # if !defined SCNxLEAST64 || @PRI_MACROS_BROKEN@ # undef SCNxLEAST64 # define SCNxLEAST64 SCNx64 # endif #endif #if !defined SCNdFAST8 || @PRI_MACROS_BROKEN@ # undef SCNdFAST8 # if INT_FAST8_MAX > INT32_MAX # define SCNdFAST8 SCNd64 # elif INT_FAST8_MAX == 0x7fff # define SCNdFAST8 "hd" # elif INT_FAST8_MAX == 0x7f # define SCNdFAST8 "hhd" # else # define SCNdFAST8 "d" # endif #endif #if !defined SCNiFAST8 || @PRI_MACROS_BROKEN@ # undef SCNiFAST8 # if INT_FAST8_MAX > INT32_MAX # define SCNiFAST8 SCNi64 # elif INT_FAST8_MAX == 0x7fff # define SCNiFAST8 "hi" # elif INT_FAST8_MAX == 0x7f # define SCNiFAST8 "hhi" # else # define SCNiFAST8 "i" # endif #endif #if !defined SCNoFAST8 || @PRI_MACROS_BROKEN@ # undef SCNoFAST8 # if UINT_FAST8_MAX > UINT32_MAX # define SCNoFAST8 SCNo64 # elif UINT_FAST8_MAX == 0xffff # define SCNoFAST8 "ho" # elif UINT_FAST8_MAX == 0xff # define SCNoFAST8 "hho" # else # define SCNoFAST8 "o" # endif #endif #if !defined SCNuFAST8 || @PRI_MACROS_BROKEN@ # undef SCNuFAST8 # if UINT_FAST8_MAX > UINT32_MAX # define SCNuFAST8 SCNu64 # elif UINT_FAST8_MAX == 0xffff # define SCNuFAST8 "hu" # elif UINT_FAST8_MAX == 0xff # define SCNuFAST8 "hhu" # else # define SCNuFAST8 "u" # endif #endif #if !defined SCNxFAST8 || @PRI_MACROS_BROKEN@ # undef SCNxFAST8 # if UINT_FAST8_MAX > UINT32_MAX # define SCNxFAST8 SCNx64 # elif UINT_FAST8_MAX == 0xffff # define SCNxFAST8 "hx" # elif UINT_FAST8_MAX == 0xff # define SCNxFAST8 "hhx" # else # define SCNxFAST8 "x" # endif #endif #if !defined SCNdFAST16 || @PRI_MACROS_BROKEN@ # undef SCNdFAST16 # if INT_FAST16_MAX > INT32_MAX # define SCNdFAST16 SCNd64 # elif INT_FAST16_MAX == 0x7fff # define SCNdFAST16 "hd" # else # define SCNdFAST16 "d" # endif #endif #if !defined SCNiFAST16 || @PRI_MACROS_BROKEN@ # undef SCNiFAST16 # if INT_FAST16_MAX > INT32_MAX # define SCNiFAST16 SCNi64 # elif INT_FAST16_MAX == 0x7fff # define SCNiFAST16 "hi" # else # define SCNiFAST16 "i" # endif #endif #if !defined SCNoFAST16 || @PRI_MACROS_BROKEN@ # undef SCNoFAST16 # if UINT_FAST16_MAX > UINT32_MAX # define SCNoFAST16 SCNo64 # elif UINT_FAST16_MAX == 0xffff # define SCNoFAST16 "ho" # else # define SCNoFAST16 "o" # endif #endif #if !defined SCNuFAST16 || @PRI_MACROS_BROKEN@ # undef SCNuFAST16 # if UINT_FAST16_MAX > UINT32_MAX # define SCNuFAST16 SCNu64 # elif UINT_FAST16_MAX == 0xffff # define SCNuFAST16 "hu" # else # define SCNuFAST16 "u" # endif #endif #if !defined SCNxFAST16 || @PRI_MACROS_BROKEN@ # undef SCNxFAST16 # if UINT_FAST16_MAX > UINT32_MAX # define SCNxFAST16 SCNx64 # elif UINT_FAST16_MAX == 0xffff # define SCNxFAST16 "hx" # else # define SCNxFAST16 "x" # endif #endif #if !defined SCNdFAST32 || @PRI_MACROS_BROKEN@ # undef SCNdFAST32 # if INT_FAST32_MAX > INT32_MAX # define SCNdFAST32 SCNd64 # else # define SCNdFAST32 "d" # endif #endif #if !defined SCNiFAST32 || @PRI_MACROS_BROKEN@ # undef SCNiFAST32 # if INT_FAST32_MAX > INT32_MAX # define SCNiFAST32 SCNi64 # else # define SCNiFAST32 "i" # endif #endif #if !defined SCNoFAST32 || @PRI_MACROS_BROKEN@ # undef SCNoFAST32 # if UINT_FAST32_MAX > UINT32_MAX # define SCNoFAST32 SCNo64 # else # define SCNoFAST32 "o" # endif #endif #if !defined SCNuFAST32 || @PRI_MACROS_BROKEN@ # undef SCNuFAST32 # if UINT_FAST32_MAX > UINT32_MAX # define SCNuFAST32 SCNu64 # else # define SCNuFAST32 "u" # endif #endif #if !defined SCNxFAST32 || @PRI_MACROS_BROKEN@ # undef SCNxFAST32 # if UINT_FAST32_MAX > UINT32_MAX # define SCNxFAST32 SCNx64 # else # define SCNxFAST32 "x" # endif #endif #ifdef INT64_MAX # if !defined SCNdFAST64 || @PRI_MACROS_BROKEN@ # undef SCNdFAST64 # define SCNdFAST64 SCNd64 # endif # if !defined SCNiFAST64 || @PRI_MACROS_BROKEN@ # undef SCNiFAST64 # define SCNiFAST64 SCNi64 # endif #endif #ifdef UINT64_MAX # if !defined SCNoFAST64 || @PRI_MACROS_BROKEN@ # undef SCNoFAST64 # define SCNoFAST64 SCNo64 # endif # if !defined SCNuFAST64 || @PRI_MACROS_BROKEN@ # undef SCNuFAST64 # define SCNuFAST64 SCNu64 # endif # if !defined SCNxFAST64 || @PRI_MACROS_BROKEN@ # undef SCNxFAST64 # define SCNxFAST64 SCNx64 # endif #endif #if !defined SCNdMAX || @PRI_MACROS_BROKEN@ # undef SCNdMAX # if @INT32_MAX_LT_INTMAX_MAX@ # define SCNdMAX SCNd64 # else # define SCNdMAX "ld" # endif #endif #if !defined SCNiMAX || @PRI_MACROS_BROKEN@ # undef SCNiMAX # if @INT32_MAX_LT_INTMAX_MAX@ # define SCNiMAX SCNi64 # else # define SCNiMAX "li" # endif #endif #if !defined SCNoMAX || @PRI_MACROS_BROKEN@ # undef SCNoMAX # if @UINT32_MAX_LT_UINTMAX_MAX@ # define SCNoMAX SCNo64 # else # define SCNoMAX "lo" # endif #endif #if !defined SCNuMAX || @PRI_MACROS_BROKEN@ # undef SCNuMAX # if @UINT32_MAX_LT_UINTMAX_MAX@ # define SCNuMAX SCNu64 # else # define SCNuMAX "lu" # endif #endif #if !defined SCNxMAX || @PRI_MACROS_BROKEN@ # undef SCNxMAX # if @UINT32_MAX_LT_UINTMAX_MAX@ # define SCNxMAX SCNx64 # else # define SCNxMAX "lx" # endif #endif #if !defined SCNdPTR || @PRI_MACROS_BROKEN@ # undef SCNdPTR # ifdef INTPTR_MAX # define SCNdPTR @PRIPTR_PREFIX@ "d" # endif #endif #if !defined SCNiPTR || @PRI_MACROS_BROKEN@ # undef SCNiPTR # ifdef INTPTR_MAX # define SCNiPTR @PRIPTR_PREFIX@ "i" # endif #endif #if !defined SCNoPTR || @PRI_MACROS_BROKEN@ # undef SCNoPTR # ifdef UINTPTR_MAX # define SCNoPTR @PRIPTR_PREFIX@ "o" # endif #endif #if !defined SCNuPTR || @PRI_MACROS_BROKEN@ # undef SCNuPTR # ifdef UINTPTR_MAX # define SCNuPTR @PRIPTR_PREFIX@ "u" # endif #endif #if !defined SCNxPTR || @PRI_MACROS_BROKEN@ # undef SCNxPTR # ifdef UINTPTR_MAX # define SCNxPTR @PRIPTR_PREFIX@ "x" # endif #endif /* 7.8.2 Functions for greatest-width integer types */ #ifdef __cplusplus extern "C" { #endif #if @GNULIB_IMAXABS@ # if !@HAVE_DECL_IMAXABS@ extern intmax_t imaxabs (intmax_t); # endif #elif defined GNULIB_POSIXCHECK # undef imaxabs # if HAVE_RAW_DECL_IMAXABS _GL_WARN_ON_USE (imaxabs, "imaxabs is unportable - " "use gnulib module imaxabs for portability"); # endif #endif #if @GNULIB_IMAXDIV@ # if !@HAVE_DECL_IMAXDIV@ # if !GNULIB_defined_imaxdiv_t typedef struct { intmax_t quot; intmax_t rem; } imaxdiv_t; # define GNULIB_defined_imaxdiv_t 1 # endif extern imaxdiv_t imaxdiv (intmax_t, intmax_t); # endif #elif defined GNULIB_POSIXCHECK # undef imaxdiv # if HAVE_RAW_DECL_IMAXDIV _GL_WARN_ON_USE (imaxdiv, "imaxdiv is unportable - " "use gnulib module imaxdiv for portability"); # endif #endif #if @GNULIB_STRTOIMAX@ # if @REPLACE_STRTOIMAX@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strtoimax # define strtoimax rpl_strtoimax # endif _GL_FUNCDECL_RPL (strtoimax, intmax_t, (const char *, char **, int) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (strtoimax, intmax_t, (const char *, char **, int)); # else # if !@HAVE_DECL_STRTOIMAX@ # undef strtoimax _GL_FUNCDECL_SYS (strtoimax, intmax_t, (const char *, char **, int) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strtoimax, intmax_t, (const char *, char **, int)); # endif _GL_CXXALIASWARN (strtoimax); #elif defined GNULIB_POSIXCHECK # undef strtoimax # if HAVE_RAW_DECL_STRTOIMAX _GL_WARN_ON_USE (strtoimax, "strtoimax is unportable - " "use gnulib module strtoimax for portability"); # endif #endif #if @GNULIB_STRTOUMAX@ # if @REPLACE_STRTOUMAX@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strtoumax # define strtoumax rpl_strtoumax # endif _GL_FUNCDECL_RPL (strtoumax, uintmax_t, (const char *, char **, int) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (strtoumax, uintmax_t, (const char *, char **, int)); # else # if !@HAVE_DECL_STRTOUMAX@ # undef strtoumax _GL_FUNCDECL_SYS (strtoumax, uintmax_t, (const char *, char **, int) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strtoumax, uintmax_t, (const char *, char **, int)); # endif _GL_CXXALIASWARN (strtoumax); #elif defined GNULIB_POSIXCHECK # undef strtoumax # if HAVE_RAW_DECL_STRTOUMAX _GL_WARN_ON_USE (strtoumax, "strtoumax is unportable - " "use gnulib module strtoumax for portability"); # endif #endif /* Don't bother defining or declaring wcstoimax and wcstoumax, since wide-character functions like this are hardly ever useful. */ #ifdef __cplusplus } #endif #endif /* !defined INTTYPES_H && !defined _GL_JUST_INCLUDE_SYSTEM_INTTYPES_H */ gnuastro-0.2.33-8a3b/bootstrapped/tests/ignore-value.h0000644000175000017500000000423413004436755017545 00000000000000/* ignore a function return without a compiler warning. -*- coding: utf-8 -*- Copyright (C) 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Jim Meyering, Eric Blake and Pádraig Brady. */ /* Use "ignore_value" to avoid a warning when using a function declared with gcc's warn_unused_result attribute, but for which you really do want to ignore the result. Traditionally, people have used a "(void)" cast to indicate that a function's return value is deliberately unused. However, if the function is declared with __attribute__((warn_unused_result)), gcc issues a warning even with the cast. Caution: most of the time, you really should heed gcc's warning, and check the return value. However, in those exceptional cases in which you're sure you know what you're doing, use this function. For the record, here's one of the ignorable warnings: "copy.c:233: warning: ignoring return value of 'fchown', declared with attribute warn_unused_result". */ #ifndef _GL_IGNORE_VALUE_H #define _GL_IGNORE_VALUE_H /* Normally casting an expression to void discards its value, but GCC versions 3.4 and newer have __attribute__ ((__warn_unused_result__)) which may cause unwanted diagnostics in that case. Use __typeof__ and __extension__ to work around the problem, if the workaround is known to be needed. */ #if 3 < __GNUC__ + (4 <= __GNUC_MINOR__) # define ignore_value(x) \ (__extension__ ({ __typeof__ (x) __x = (x); (void) __x; })) #else # define ignore_value(x) ((void) (x)) #endif #endif gnuastro-0.2.33-8a3b/bootstrapped/tests/test-getopt_long.h0000644000175000017500000017552413004436755020461 00000000000000/* Test of command line argument processing. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ static int a_seen; static int b_seen; static int q_seen; static const struct option long_options_required[] = { { "alpha", no_argument, NULL, 'a' }, { "beta", no_argument, &b_seen, 1 }, { "prune", required_argument, NULL, 'p' }, { "quetsche", required_argument, &q_seen, 1 }, { "xtremely-",no_argument, NULL, 1003 }, { "xtra", no_argument, NULL, 1001 }, { "xtreme", no_argument, NULL, 1002 }, { "xtremely", no_argument, NULL, 1003 }, { NULL, 0, NULL, 0 } }; static const struct option long_options_optional[] = { { "alpha", no_argument, NULL, 'a' }, { "beta", no_argument, &b_seen, 1 }, { "prune", optional_argument, NULL, 'p' }, { "quetsche", optional_argument, &q_seen, 1 }, { NULL, 0, NULL, 0 } }; static void getopt_long_loop (int argc, const char **argv, const char *options, const struct option *long_options, const char **p_value, const char **q_value, int *non_options_count, const char **non_options, int *unrecognized) { int option_index = -1; int c; opterr = 0; q_seen = 0; while ((c = getopt_long (argc, (char **) argv, options, long_options, &option_index)) != -1) { switch (c) { case 0: /* An option with a non-NULL flag pointer was processed. */ if (q_seen) *q_value = optarg; break; case 'a': a_seen++; break; case 'b': b_seen = 1; break; case 'p': *p_value = optarg; break; case 'q': *q_value = optarg; break; case '\1': /* Must only happen with option '-' at the beginning. */ ASSERT (options[0] == '-'); non_options[(*non_options_count)++] = optarg; break; case ':': /* Must only happen with option ':' at the beginning. */ ASSERT (options[0] == ':' || ((options[0] == '-' || options[0] == '+') && options[1] == ':')); /* fall through */ case '?': *unrecognized = optopt; break; default: *unrecognized = c; break; } } } /* Reduce casting, so we can use string literals elsewhere. getopt_long takes an array of char*, but luckily does not modify those elements, so we can pass const char*. */ static int do_getopt_long (int argc, const char **argv, const char *shortopts, const struct option *longopts, int *longind) { return getopt_long (argc, (char **) argv, shortopts, longopts, longind); } static void test_getopt_long (void) { int start; /* Test disambiguation of options. */ { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--x"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xt"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xtr"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xtra"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == 1001); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xtre"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xtrem"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xtreme"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == 1002); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xtremel"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == 1003); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xtremely"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == 1003); } /* Check that -W handles unknown options. */ { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "W;", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 'W'); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-Wunknown"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "W;", long_options_required, &option_index); /* glibc and BSD behave differently here, but for now, we allow both behaviors since W support is not frequently used. */ if (c == '?') { ASSERT (optopt == 0); ASSERT (optarg == NULL); } else { ASSERT (c == 'W'); ASSERT (strcmp (optarg, "unknown") == 0); } } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc++] = "unknown"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "W;", long_options_required, &option_index); /* glibc and BSD behave differently here, but for now, we allow both behaviors since W support is not frequently used. */ if (c == '?') { ASSERT (optopt == 0); ASSERT (optarg == NULL); } else { ASSERT (c == 'W'); ASSERT (strcmp (optarg, "unknown") == 0); } } /* Test that 'W' does not dump core: http://sourceware.org/bugzilla/show_bug.cgi?id=12922 */ { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc++] = "dummy"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "W;", NULL, &option_index); ASSERT (c == 'W'); ASSERT (optind == 2); } /* Test processing of boolean short options. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-a"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-b"; argv[argc++] = "-a"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-ba"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-ab"; argv[argc++] = "-a"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 2); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } /* Test processing of boolean long options. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--alpha"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--beta"; argv[argc++] = "--alpha"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--alpha"; argv[argc++] = "--beta"; argv[argc++] = "--alpha"; argv[argc++] = "--beta"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 2); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); } /* Test processing of boolean long options via -W. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-Walpha"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abW;", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc++] = "beta"; argv[argc++] = "-W"; argv[argc++] = "alpha"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "aW;b", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-Walpha"; argv[argc++] = "-Wbeta"; argv[argc++] = "-Walpha"; argv[argc++] = "-Wbeta"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "W;ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 2); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); } /* Test processing of short options with arguments. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-pfoo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-ab"; argv[argc++] = "-q"; argv[argc++] = "baz"; argv[argc++] = "-pfoo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value != NULL && strcmp (q_value, "baz") == 0); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); } /* Test processing of long options with arguments. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--p=foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--p"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-ab"; argv[argc++] = "--q"; argv[argc++] = "baz"; argv[argc++] = "--p=foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value != NULL && strcmp (q_value, "baz") == 0); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); } /* Test processing of long options with arguments via -W. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-Wp=foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p:q:W;", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc++] = "p"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p:W;q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-ab"; argv[argc++] = "-Wq"; argv[argc++] = "baz"; argv[argc++] = "-W"; argv[argc++] = "p=foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "W;abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value != NULL && strcmp (q_value, "baz") == 0); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 6); } /* Test processing of short options with optional arguments. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-pfoo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } /* Test processing of long options with optional arguments. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--p=foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--p"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--p="; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && *p_value == '\0'); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--p"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } /* Test processing of long options with optional arguments via -W. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-Wp=foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::q::W;", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-Wp"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::q::W;", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-Wp="; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "W;p::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && *p_value == '\0'); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc++] = "p="; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "W;p::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && *p_value == '\0'); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc++] = "p"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "W;abp::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); /* ASSERT (p_value == NULL); */ ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); } /* Check that invalid options are recognized. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-x"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'x'); ASSERT (optind == 5); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-:"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == ':'); ASSERT (optind == 5); } /* Check that unexpected arguments are recognized. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "--a="; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'a'); ASSERT (optind == 4); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "--b="; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); /* When flag is non-zero, glibc sets optopt anyway, but BSD leaves optopt unchanged. */ ASSERT (unrecognized == 1 || unrecognized == 0); ASSERT (optind == 4); } /* Check that by default, non-options arguments are moved to the end. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "donald") == 0); ASSERT (strcmp (argv[5], "duck") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); } /* Check that '--' ends the argument processing. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[20]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "--"; argv[argc++] = "-b"; argv[argc++] = "foo"; argv[argc++] = "-q"; argv[argc++] = "johnny"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "--") == 0); ASSERT (strcmp (argv[5], "donald") == 0); ASSERT (strcmp (argv[6], "duck") == 0); ASSERT (strcmp (argv[7], "-b") == 0); ASSERT (strcmp (argv[8], "foo") == 0); ASSERT (strcmp (argv[9], "-q") == 0); ASSERT (strcmp (argv[10], "johnny") == 0); ASSERT (strcmp (argv[11], "bar") == 0); ASSERT (argv[12] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); } /* Check that the '-' flag causes non-options to be returned in order. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "-abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 3); ASSERT (strcmp (non_options[0], "donald") == 0); ASSERT (strcmp (non_options[1], "duck") == 0); ASSERT (strcmp (non_options[2], "bar") == 0); ASSERT (unrecognized == 0); ASSERT (optind == 7); } /* Check that '--' ends the argument processing. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[20]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "--"; argv[argc++] = "-b"; argv[argc++] = "foo"; argv[argc++] = "-q"; argv[argc++] = "johnny"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "-abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "--") == 0); ASSERT (strcmp (argv[7], "-b") == 0); ASSERT (strcmp (argv[8], "foo") == 0); ASSERT (strcmp (argv[9], "-q") == 0); ASSERT (strcmp (argv[10], "johnny") == 0); ASSERT (strcmp (argv[11], "bar") == 0); ASSERT (argv[12] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); if (non_options_count == 2) { /* glibc behaviour. */ ASSERT (non_options_count == 2); ASSERT (strcmp (non_options[0], "donald") == 0); ASSERT (strcmp (non_options[1], "duck") == 0); ASSERT (unrecognized == 0); ASSERT (optind == 7); } else { /* Another valid behaviour. */ ASSERT (non_options_count == 7); ASSERT (strcmp (non_options[0], "donald") == 0); ASSERT (strcmp (non_options[1], "duck") == 0); ASSERT (strcmp (non_options[2], "-b") == 0); ASSERT (strcmp (non_options[3], "foo") == 0); ASSERT (strcmp (non_options[4], "-q") == 0); ASSERT (strcmp (non_options[5], "johnny") == 0); ASSERT (strcmp (non_options[6], "bar") == 0); ASSERT (unrecognized == 0); ASSERT (optind == 12); } } /* Check that the '-' flag has to come first. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:-", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "donald") == 0); ASSERT (strcmp (argv[5], "duck") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); } /* Check that the '+' flag causes the first non-option to terminate the loop. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "+abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-+"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "+abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == '+'); ASSERT (optind == 2); } /* Check that '--' ends the argument processing. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[20]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "--"; argv[argc++] = "-b"; argv[argc++] = "foo"; argv[argc++] = "-q"; argv[argc++] = "johnny"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "+abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "--") == 0); ASSERT (strcmp (argv[7], "-b") == 0); ASSERT (strcmp (argv[8], "foo") == 0); ASSERT (strcmp (argv[9], "-q") == 0); ASSERT (strcmp (argv[10], "johnny") == 0); ASSERT (strcmp (argv[11], "bar") == 0); ASSERT (argv[12] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); } /* Check that the '+' flag has to come first. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:+", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "donald") == 0); ASSERT (strcmp (argv[5], "duck") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); } } /* Test behavior of getopt_long when POSIXLY_CORRECT is set in the environment. Options with optional arguments should not change behavior just because of an environment variable. http://lists.gnu.org/archive/html/bug-m4/2006-09/msg00028.html */ static void test_getopt_long_posix (void) { int start; /* Check that POSIXLY_CORRECT stops parsing the same as leading '+'. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); } /* Check that POSIXLY_CORRECT doesn't change optional arguments. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } /* Check that leading - still sees options after non-options. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-a"; argv[argc++] = "billy"; argv[argc++] = "-b"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "-ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 1); ASSERT (strcmp (non_options[0], "billy") == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); } } /* Reduce casting, so we can use string literals elsewhere. getopt_long_only takes an array of char*, but luckily does not modify those elements, so we can pass const char*. */ static int do_getopt_long_only (int argc, const char **argv, const char *shortopts, const struct option *longopts, int *longind) { return getopt_long_only (argc, (char **) argv, shortopts, longopts, longind); } static void test_getopt_long_only (void) { /* Test disambiguation of options. */ { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-x"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-x"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "abx", long_options_required, &option_index); ASSERT (c == 'x'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--x"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "abx", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-b"; argv[argc] = NULL; optind = 1; opterr = 0; b_seen = 0; c = do_getopt_long_only (argc, argv, "abx", long_options_required, &option_index); ASSERT (c == 'b'); ASSERT (b_seen == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--b"; argv[argc] = NULL; optind = 1; opterr = 0; b_seen = 0; c = do_getopt_long_only (argc, argv, "abx", long_options_required, &option_index); ASSERT (c == 0); ASSERT (b_seen == 1); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-xt"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-xt"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "abx", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-xtra"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == 1001); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-xtreme"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "abx:", long_options_required, &option_index); ASSERT (c == 1002); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-xtremel"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "ab", long_options_required, &option_index); /* glibc getopt_long_only is intentionally different from getopt_long when handling a prefix that is common to two spellings, when both spellings have the same option directives. BSD getopt_long_only treats both cases the same. */ ASSERT (c == 1003 || c == '?'); ASSERT (optind == 2); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-xtremel"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "abx::", long_options_required, &option_index); /* glibc getopt_long_only is intentionally different from getopt_long when handling a prefix that is common to two spellings, when both spellings have the same option directives. BSD getopt_long_only treats both cases the same. */ ASSERT (c == 1003 || c == '?'); ASSERT (optind == 2); ASSERT (optarg == NULL); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-xtras"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "abx::", long_options_required, &option_index); ASSERT (c == 'x'); ASSERT (strcmp (optarg, "tras") == 0); } } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-getopt.h0000644000175000017500000012566113004436755017437 00000000000000/* Test of command line argument processing. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ #include /* The glibc/gnulib implementation of getopt supports setting optind = 0, but not all other implementations do. This matters for getopt. But for getopt_long, we require GNU compatibility. */ #if defined __GETOPT_PREFIX || (__GLIBC__ >= 2 && !defined __UCLIBC__) # define OPTIND_MIN 0 #elif HAVE_DECL_OPTRESET # define OPTIND_MIN (optreset = 1) #else # define OPTIND_MIN 1 #endif static void getopt_loop (int argc, const char **argv, const char *options, int *a_seen, int *b_seen, const char **p_value, const char **q_value, int *non_options_count, const char **non_options, int *unrecognized, bool *message_issued) { int c; int pos = ftell (stderr); while ((c = getopt (argc, (char **) argv, options)) != -1) { switch (c) { case 'a': (*a_seen)++; break; case 'b': (*b_seen)++; break; case 'p': *p_value = optarg; break; case 'q': *q_value = optarg; break; case '\1': /* Must only happen with option '-' at the beginning. */ ASSERT (options[0] == '-'); non_options[(*non_options_count)++] = optarg; break; case ':': /* Must only happen with option ':' at the beginning. */ ASSERT (options[0] == ':' || ((options[0] == '-' || options[0] == '+') && options[1] == ':')); /* fall through */ case '?': *unrecognized = optopt; break; default: *unrecognized = c; break; } } *message_issued = pos < ftell (stderr); } static void test_getopt (void) { int start; bool posixly = !!getenv ("POSIXLY_CORRECT"); /* See comment in getopt.c: glibc gets a LSB-compliant getopt. Standalone applications get a POSIX-compliant getopt. */ #if defined __GETOPT_PREFIX || !(__GLIBC__ >= 2 || defined __MINGW32__) /* Using getopt from gnulib or from a non-glibc system. */ posixly = true; #endif /* Test processing of boolean options. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-a"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "ab", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-b"; argv[argc++] = "-a"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "ab", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-ba"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "ab", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-ab"; argv[argc++] = "-a"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "ab", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 2); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); ASSERT (!output); } /* Test processing of options with arguments. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-pfoo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "p:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "p:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-ab"; argv[argc++] = "-q"; argv[argc++] = "baz"; argv[argc++] = "-pfoo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value != NULL && strcmp (q_value, "baz") == 0); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); ASSERT (!output); } #if GNULIB_TEST_GETOPT_GNU /* Test processing of options with optional arguments. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-pfoo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "p::q::", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "p::q::", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "abp::q::", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); ASSERT (!output); } #endif /* GNULIB_TEST_GETOPT_GNU */ /* Check that invalid options are recognized; and that both opterr and leading ':' can silence output. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-x"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 42; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'x'); ASSERT (optind == 5); ASSERT (output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-x"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 0; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'x'); ASSERT (optind == 5); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-x"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, ":abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'x'); ASSERT (optind == 5); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-:"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 42; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == ':'); ASSERT (optind == 5); ASSERT (output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-:"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 0; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == ':'); ASSERT (optind == 5); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-:"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, ":abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == ':'); ASSERT (optind == 5); ASSERT (!output); } /* Check for missing argument behavior. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-ap"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'p'); ASSERT (optind == 2); ASSERT (output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-ap"; argv[argc] = NULL; optind = start; opterr = 0; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'p'); ASSERT (optind == 2); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-ap"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, ":abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'p'); ASSERT (optind == 2); ASSERT (!output); } /* Check that by default, non-options arguments are moved to the end. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); if (posixly) { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); ASSERT (!output); } else { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "donald") == 0); ASSERT (strcmp (argv[5], "duck") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); ASSERT (!output); } } /* Check that '--' ends the argument processing. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[20]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "--"; argv[argc++] = "-b"; argv[argc++] = "foo"; argv[argc++] = "-q"; argv[argc++] = "johnny"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); if (posixly) { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "--") == 0); ASSERT (strcmp (argv[7], "-b") == 0); ASSERT (strcmp (argv[8], "foo") == 0); ASSERT (strcmp (argv[9], "-q") == 0); ASSERT (strcmp (argv[10], "johnny") == 0); ASSERT (strcmp (argv[11], "bar") == 0); ASSERT (argv[12] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); ASSERT (!output); } else { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "--") == 0); ASSERT (strcmp (argv[5], "donald") == 0); ASSERT (strcmp (argv[6], "duck") == 0); ASSERT (strcmp (argv[7], "-b") == 0); ASSERT (strcmp (argv[8], "foo") == 0); ASSERT (strcmp (argv[9], "-q") == 0); ASSERT (strcmp (argv[10], "johnny") == 0); ASSERT (strcmp (argv[11], "bar") == 0); ASSERT (argv[12] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); ASSERT (!output); } } #if GNULIB_TEST_GETOPT_GNU /* Check that the '-' flag causes non-options to be returned in order. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "-abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 3); ASSERT (strcmp (non_options[0], "donald") == 0); ASSERT (strcmp (non_options[1], "duck") == 0); ASSERT (strcmp (non_options[2], "bar") == 0); ASSERT (unrecognized == 0); ASSERT (optind == 7); ASSERT (!output); } /* Check that '--' ends the argument processing. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[20]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "--"; argv[argc++] = "-b"; argv[argc++] = "foo"; argv[argc++] = "-q"; argv[argc++] = "johnny"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "-abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "--") == 0); ASSERT (strcmp (argv[7], "-b") == 0); ASSERT (strcmp (argv[8], "foo") == 0); ASSERT (strcmp (argv[9], "-q") == 0); ASSERT (strcmp (argv[10], "johnny") == 0); ASSERT (strcmp (argv[11], "bar") == 0); ASSERT (argv[12] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (!output); if (non_options_count == 2) { /* glibc behaviour. */ ASSERT (non_options_count == 2); ASSERT (strcmp (non_options[0], "donald") == 0); ASSERT (strcmp (non_options[1], "duck") == 0); ASSERT (unrecognized == 0); ASSERT (optind == 7); } else { /* Another valid behaviour. */ ASSERT (non_options_count == 7); ASSERT (strcmp (non_options[0], "donald") == 0); ASSERT (strcmp (non_options[1], "duck") == 0); ASSERT (strcmp (non_options[2], "-b") == 0); ASSERT (strcmp (non_options[3], "foo") == 0); ASSERT (strcmp (non_options[4], "-q") == 0); ASSERT (strcmp (non_options[5], "johnny") == 0); ASSERT (strcmp (non_options[6], "bar") == 0); ASSERT (unrecognized == 0); ASSERT (optind == 12); } } /* Check that the '-' flag has to come first. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "abp:q:-", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); if (posixly) { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); ASSERT (!output); } else { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "donald") == 0); ASSERT (strcmp (argv[5], "duck") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); ASSERT (!output); } } /* Check that the '+' flag causes the first non-option to terminate the loop. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "+abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-+"; argv[argc] = NULL; optind = start; getopt_loop (argc, argv, "+abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == '+'); ASSERT (optind == 2); ASSERT (output); } /* Check that '--' ends the argument processing. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[20]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "--"; argv[argc++] = "-b"; argv[argc++] = "foo"; argv[argc++] = "-q"; argv[argc++] = "johnny"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "+abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "--") == 0); ASSERT (strcmp (argv[7], "-b") == 0); ASSERT (strcmp (argv[8], "foo") == 0); ASSERT (strcmp (argv[9], "-q") == 0); ASSERT (strcmp (argv[10], "johnny") == 0); ASSERT (strcmp (argv[11], "bar") == 0); ASSERT (argv[12] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); ASSERT (!output); } #endif /* GNULIB_TEST_GETOPT_GNU */ /* Check that the '+' flag has to come first. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "abp:q:+", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); if (posixly) { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); ASSERT (!output); } else { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "donald") == 0); ASSERT (strcmp (argv[5], "duck") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); ASSERT (!output); } } #if GNULIB_TEST_GETOPT_GNU /* If GNU extensions are supported, require compliance with POSIX interpretation on leading '+' behavior. http://austingroupbugs.net/view.php?id=191 */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "+:abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc] = NULL; optind = start; getopt_loop (argc, argv, "+:abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'p'); ASSERT (optind == 2); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-b"; argv[argc++] = "-p"; argv[argc] = NULL; optind = start; getopt_loop (argc, argv, "+:abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 0); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'p'); ASSERT (optind == 3); ASSERT (!output); } /* Check that 'W' does not dump core: http://sourceware.org/bugzilla/show_bug.cgi?id=12922 Technically, POSIX says the presence of ';' in the opt-string gives unspecified behavior, so we only test this when GNU compliance is desired. */ for (start = OPTIND_MIN; start <= 1; start++) { int argc = 0; const char *argv[10]; int pos = ftell (stderr); argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc++] = "dummy"; argv[argc] = NULL; optind = start; opterr = 1; ASSERT (getopt (argc, (char **) argv, "W;") == 'W'); ASSERT (ftell (stderr) == pos); ASSERT (optind == 2); } #endif /* GNULIB_TEST_GETOPT_GNU */ } gnuastro-0.2.33-8a3b/bootstrapped/tests/fpucw.h0000644000175000017500000001116213004436755016272 00000000000000/* Manipulating the FPU control word. -*- coding: utf-8 -*- Copyright (C) 2007-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2007. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _FPUCW_H #define _FPUCW_H /* The i386 floating point hardware (the 387 compatible FPU, not the modern SSE/SSE2 hardware) has a controllable rounding precision. It is specified through the 'PC' bits in the FPU control word ('fctrl' register). (See the GNU libc i386 header for details.) On some platforms, such as Linux or Solaris, the default precision setting is set to "extended precision". This means that 'long double' instructions operate correctly, but 'double' computations often produce slightly different results as on strictly IEEE 754 conforming systems. On some platforms, such as NetBSD, the default precision is set to "double precision". This means that 'long double' instructions will operate only as 'double', i.e. lead to wrong results. Similarly on FreeBSD 6.4, at least for the division of 'long double' numbers. The FPU control word is under control of the application, i.e. it is not required to be set either way by the ABI. (In fact, the i386 ABI http://refspecs.freestandards.org/elf/abi386-4.pdf page 3-12 = page 38 is not clear about it. But in any case, gcc treats the control word like a "preserved" register: it emits code that assumes that the control word is preserved across calls, and it restores the control word at the end of functions that modify it.) See Vincent Lefèvre's page http://www.vinc17.org/research/extended.en.html for a good explanation. See http://www.uwsg.iu.edu/hypermail/linux/kernel/0103.0/0453.html for some argumentation which setting should be the default. */ /* This header file provides the following facilities: fpucw_t integral type holding the value of 'fctrl' FPU_PC_MASK bit mask denoting the precision control FPU_PC_DOUBLE precision control for 53 bits mantissa FPU_PC_EXTENDED precision control for 64 bits mantissa GET_FPUCW () yields the current FPU control word SET_FPUCW (word) sets the FPU control word DECL_LONG_DOUBLE_ROUNDING variable declaration for BEGIN/END_LONG_DOUBLE_ROUNDING BEGIN_LONG_DOUBLE_ROUNDING () starts a sequence of instructions with 'long double' safe operation precision END_LONG_DOUBLE_ROUNDING () ends a sequence of instructions with 'long double' safe operation precision */ /* Inline assembler like this works only with GNU C. */ #if (defined __i386__ || defined __x86_64__) && defined __GNUC__ typedef unsigned short fpucw_t; /* glibc calls this fpu_control_t */ # define FPU_PC_MASK 0x0300 # define FPU_PC_DOUBLE 0x200 /* glibc calls this _FPU_DOUBLE */ # define FPU_PC_EXTENDED 0x300 /* glibc calls this _FPU_EXTENDED */ # define GET_FPUCW() \ ({ fpucw_t _cw; \ __asm__ __volatile__ ("fnstcw %0" : "=m" (*&_cw)); \ _cw; \ }) # define SET_FPUCW(word) \ (void)({ fpucw_t _ncw = (word); \ __asm__ __volatile__ ("fldcw %0" : : "m" (*&_ncw)); \ }) # define DECL_LONG_DOUBLE_ROUNDING \ fpucw_t oldcw; # define BEGIN_LONG_DOUBLE_ROUNDING() \ (void)(oldcw = GET_FPUCW (), \ SET_FPUCW ((oldcw & ~FPU_PC_MASK) | FPU_PC_EXTENDED)) # define END_LONG_DOUBLE_ROUNDING() \ SET_FPUCW (oldcw) #else typedef unsigned int fpucw_t; # define FPU_PC_MASK 0 # define FPU_PC_DOUBLE 0 # define FPU_PC_EXTENDED 0 # define GET_FPUCW() 0 # define SET_FPUCW(word) (void)(word) # define DECL_LONG_DOUBLE_ROUNDING # define BEGIN_LONG_DOUBLE_ROUNDING() # define END_LONG_DOUBLE_ROUNDING() #endif #endif /* _FPUCW_H */ gnuastro-0.2.33-8a3b/bootstrapped/tests/flexmember.h0000644000175000017500000000334613004436755017301 00000000000000/* Sizes of structs with flexible array members. Copyright 2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . Written by Paul Eggert. */ #include /* Nonzero multiple of alignment of TYPE, suitable for FLEXSIZEOF below. On older platforms without _Alignof, use a pessimistic bound that is safe in practice even if FLEXIBLE_ARRAY_MEMBER is 1. On newer platforms, use _Alignof to get a tighter bound. */ #if !defined __STDC_VERSION__ || __STDC_VERSION__ < 201112 # define FLEXALIGNOF(type) (sizeof (type) & ~ (sizeof (type) - 1)) #else # define FLEXALIGNOF(type) _Alignof (type) #endif /* Upper bound on the size of a struct of type TYPE with a flexible array member named MEMBER that is followed by N bytes of other data. This is not simply sizeof (TYPE) + N, since it may require alignment on unusually picky C11 platforms, and FLEXIBLE_ARRAY_MEMBER may be 1 on pre-C11 platforms. Yield a value less than N if and only if arithmetic overflow occurs. */ #define FLEXSIZEOF(type, member, n) \ ((offsetof (type, member) + FLEXALIGNOF (type) - 1 + (n)) \ & ~ (FLEXALIGNOF (type) - 1)) gnuastro-0.2.33-8a3b/bootstrapped/tests/fd-hook.h0000644000175000017500000001135113004436755016475 00000000000000/* Hook for making making file descriptor functions close(), ioctl() extensible. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef FD_HOOK_H #define FD_HOOK_H #ifdef __cplusplus extern "C" { #endif /* Currently, this entire code is only needed for the handling of sockets on native Windows platforms. */ #if WINDOWS_SOCKETS /* Type of function that closes FD. */ typedef int (*gl_close_fn) (int fd); /* Type of function that applies a control request to FD. */ typedef int (*gl_ioctl_fn) (int fd, int request, void *arg); /* An element of the list of file descriptor hooks. In CLOS (Common Lisp Object System) speak, it consists of an "around" method for the close() function and an "around" method for the ioctl() function. The fields of this structure are considered private. */ struct fd_hook { /* Doubly linked list. */ struct fd_hook *private_next; struct fd_hook *private_prev; /* Function that treats the types of FD that it knows about and calls execute_close_hooks (REMAINING_LIST, PRIMARY, FD) as a fallback. */ int (*private_close_fn) (const struct fd_hook *remaining_list, gl_close_fn primary, int fd); /* Function that treats the types of FD that it knows about and calls execute_ioctl_hooks (REMAINING_LIST, PRIMARY, FD, REQUEST, ARG) as a fallback. */ int (*private_ioctl_fn) (const struct fd_hook *remaining_list, gl_ioctl_fn primary, int fd, int request, void *arg); }; /* This type of function closes FD, applying special knowledge for the FD types it knows about, and calls execute_close_hooks (REMAINING_LIST, PRIMARY, FD) for the other FD types. In CLOS speak, REMAINING_LIST is the remaining list of "around" methods, and PRIMARY is the "primary" method for close(). */ typedef int (*close_hook_fn) (const struct fd_hook *remaining_list, gl_close_fn primary, int fd); /* Execute the close hooks in REMAINING_LIST, with PRIMARY as "primary" method. Return 0 or -1, like close() would do. */ extern int execute_close_hooks (const struct fd_hook *remaining_list, gl_close_fn primary, int fd); /* Execute all close hooks, with PRIMARY as "primary" method. Return 0 or -1, like close() would do. */ extern int execute_all_close_hooks (gl_close_fn primary, int fd); /* This type of function applies a control request to FD, applying special knowledge for the FD types it knows about, and calls execute_ioctl_hooks (REMAINING_LIST, PRIMARY, FD, REQUEST, ARG) for the other FD types. In CLOS speak, REMAINING_LIST is the remaining list of "around" methods, and PRIMARY is the "primary" method for ioctl(). */ typedef int (*ioctl_hook_fn) (const struct fd_hook *remaining_list, gl_ioctl_fn primary, int fd, int request, void *arg); /* Execute the ioctl hooks in REMAINING_LIST, with PRIMARY as "primary" method. Return 0 or -1, like ioctl() would do. */ extern int execute_ioctl_hooks (const struct fd_hook *remaining_list, gl_ioctl_fn primary, int fd, int request, void *arg); /* Execute all ioctl hooks, with PRIMARY as "primary" method. Return 0 or -1, like ioctl() would do. */ extern int execute_all_ioctl_hooks (gl_ioctl_fn primary, int fd, int request, void *arg); /* Add a function pair to the list of file descriptor hooks. CLOSE_HOOK and IOCTL_HOOK may be NULL, indicating no change. The LINK variable points to a piece of memory which is guaranteed to be accessible until the corresponding call to unregister_fd_hook. */ extern void register_fd_hook (close_hook_fn close_hook, ioctl_hook_fn ioctl_hook, struct fd_hook *link); /* Removes a hook from the list of file descriptor hooks. */ extern void unregister_fd_hook (struct fd_hook *link); #endif #ifdef __cplusplus } #endif #endif /* FD_HOOK_H */ gnuastro-0.2.33-8a3b/bootstrapped/tests/fcntl.in.h0000644000175000017500000002355513004436755016672 00000000000000/* Like , but with non-working flags defined to 0. Copyright (C) 2006-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* written by Paul Eggert */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if defined __need_system_fcntl_h /* Special invocation convention. */ /* Needed before . May also define off_t to a 64-bit type on native Windows. */ #include /* On some systems other than glibc, is a prerequisite of . On glibc systems, we would like to avoid namespace pollution. But on glibc systems, includes inside an extern "C" { ... } block, which leads to errors in C++ mode with the overridden from gnulib. These errors are known to be gone with g++ version >= 4.3. */ #if !(defined __GLIBC__ || defined __UCLIBC__) || (defined __cplusplus && defined GNULIB_NAMESPACE && (defined __ICC || !(__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 3)))) # include #endif #@INCLUDE_NEXT@ @NEXT_FCNTL_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_FCNTL_H /* Needed before . May also define off_t to a 64-bit type on native Windows. */ #include /* On some systems other than glibc, is a prerequisite of . On glibc systems, we would like to avoid namespace pollution. But on glibc systems, includes inside an extern "C" { ... } block, which leads to errors in C++ mode with the overridden from gnulib. These errors are known to be gone with g++ version >= 4.3. */ #if !(defined __GLIBC__ || defined __UCLIBC__) || (defined __cplusplus && defined GNULIB_NAMESPACE && (defined __ICC || !(__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 3)))) # include #endif /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_FCNTL_H@ #ifndef _@GUARD_PREFIX@_FCNTL_H #define _@GUARD_PREFIX@_FCNTL_H #ifndef __GLIBC__ /* Avoid namespace pollution on glibc systems. */ # include #endif /* Native Windows platforms declare open(), creat() in . */ #if (@GNULIB_OPEN@ || defined GNULIB_POSIXCHECK) \ && ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) # include #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Declare overridden functions. */ #if @GNULIB_FCNTL@ # if @REPLACE_FCNTL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fcntl # define fcntl rpl_fcntl # endif _GL_FUNCDECL_RPL (fcntl, int, (int fd, int action, ...)); _GL_CXXALIAS_RPL (fcntl, int, (int fd, int action, ...)); # else # if !@HAVE_FCNTL@ _GL_FUNCDECL_SYS (fcntl, int, (int fd, int action, ...)); # endif _GL_CXXALIAS_SYS (fcntl, int, (int fd, int action, ...)); # endif _GL_CXXALIASWARN (fcntl); #elif defined GNULIB_POSIXCHECK # undef fcntl # if HAVE_RAW_DECL_FCNTL _GL_WARN_ON_USE (fcntl, "fcntl is not always POSIX compliant - " "use gnulib module fcntl for portability"); # endif #endif #if @GNULIB_OPEN@ # if @REPLACE_OPEN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef open # define open rpl_open # endif _GL_FUNCDECL_RPL (open, int, (const char *filename, int flags, ...) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (open, int, (const char *filename, int flags, ...)); # else _GL_CXXALIAS_SYS (open, int, (const char *filename, int flags, ...)); # endif /* On HP-UX 11, in C++ mode, open() is defined as an inline function with a default argument. _GL_CXXALIASWARN does not work in this case. */ # if !defined __hpux _GL_CXXALIASWARN (open); # endif #elif defined GNULIB_POSIXCHECK # undef open /* Assume open is always declared. */ _GL_WARN_ON_USE (open, "open is not always POSIX compliant - " "use gnulib module open for portability"); #endif #if @GNULIB_OPENAT@ # if @REPLACE_OPENAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef openat # define openat rpl_openat # endif _GL_FUNCDECL_RPL (openat, int, (int fd, char const *file, int flags, /* mode_t mode */ ...) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (openat, int, (int fd, char const *file, int flags, /* mode_t mode */ ...)); # else # if !@HAVE_OPENAT@ _GL_FUNCDECL_SYS (openat, int, (int fd, char const *file, int flags, /* mode_t mode */ ...) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (openat, int, (int fd, char const *file, int flags, /* mode_t mode */ ...)); # endif _GL_CXXALIASWARN (openat); #elif defined GNULIB_POSIXCHECK # undef openat # if HAVE_RAW_DECL_OPENAT _GL_WARN_ON_USE (openat, "openat is not portable - " "use gnulib module openat for portability"); # endif #endif /* Fix up the FD_* macros, only known to be missing on mingw. */ #ifndef FD_CLOEXEC # define FD_CLOEXEC 1 #endif /* Fix up the supported F_* macros. Intentionally leave other F_* macros undefined. Only known to be missing on mingw. */ #ifndef F_DUPFD_CLOEXEC # define F_DUPFD_CLOEXEC 0x40000000 /* Witness variable: 1 if gnulib defined F_DUPFD_CLOEXEC, 0 otherwise. */ # define GNULIB_defined_F_DUPFD_CLOEXEC 1 #else # define GNULIB_defined_F_DUPFD_CLOEXEC 0 #endif #ifndef F_DUPFD # define F_DUPFD 1 #endif #ifndef F_GETFD # define F_GETFD 2 #endif /* Fix up the O_* macros. */ /* AIX 7.1 with XL C 12.1 defines O_CLOEXEC, O_NOFOLLOW, and O_TTY_INIT to values outside 'int' range, so omit these misdefinitions. But avoid namespace pollution on non-AIX systems. */ #ifdef _AIX # include # if defined O_CLOEXEC && ! (INT_MIN <= O_CLOEXEC && O_CLOEXEC <= INT_MAX) # undef O_CLOEXEC # endif # if defined O_NOFOLLOW && ! (INT_MIN <= O_NOFOLLOW && O_NOFOLLOW <= INT_MAX) # undef O_NOFOLLOW # endif # if defined O_TTY_INIT && ! (INT_MIN <= O_TTY_INIT && O_TTY_INIT <= INT_MAX) # undef O_TTY_INIT # endif #endif #if !defined O_DIRECT && defined O_DIRECTIO /* Tru64 spells it 'O_DIRECTIO'. */ # define O_DIRECT O_DIRECTIO #endif #if !defined O_CLOEXEC && defined O_NOINHERIT /* Mingw spells it 'O_NOINHERIT'. */ # define O_CLOEXEC O_NOINHERIT #endif #ifndef O_CLOEXEC # define O_CLOEXEC 0 #endif #ifndef O_DIRECT # define O_DIRECT 0 #endif #ifndef O_DIRECTORY # define O_DIRECTORY 0 #endif #ifndef O_DSYNC # define O_DSYNC 0 #endif #ifndef O_EXEC # define O_EXEC O_RDONLY /* This is often close enough in older systems. */ #endif #ifndef O_IGNORE_CTTY # define O_IGNORE_CTTY 0 #endif #ifndef O_NDELAY # define O_NDELAY 0 #endif #ifndef O_NOATIME # define O_NOATIME 0 #endif #ifndef O_NONBLOCK # define O_NONBLOCK O_NDELAY #endif /* If the gnulib module 'nonblocking' is in use, guarantee a working non-zero value of O_NONBLOCK. Otherwise, O_NONBLOCK is defined (above) to O_NDELAY or to 0 as fallback. */ #if @GNULIB_NONBLOCKING@ # if O_NONBLOCK # define GNULIB_defined_O_NONBLOCK 0 # else # define GNULIB_defined_O_NONBLOCK 1 # undef O_NONBLOCK # define O_NONBLOCK 0x40000000 # endif #endif #ifndef O_NOCTTY # define O_NOCTTY 0 #endif #ifndef O_NOFOLLOW # define O_NOFOLLOW 0 #endif #ifndef O_NOLINK # define O_NOLINK 0 #endif #ifndef O_NOLINKS # define O_NOLINKS 0 #endif #ifndef O_NOTRANS # define O_NOTRANS 0 #endif #ifndef O_RSYNC # define O_RSYNC 0 #endif #ifndef O_SEARCH # define O_SEARCH O_RDONLY /* This is often close enough in older systems. */ #endif #ifndef O_SYNC # define O_SYNC 0 #endif #ifndef O_TTY_INIT # define O_TTY_INIT 0 #endif #if ~O_ACCMODE & (O_RDONLY | O_WRONLY | O_RDWR | O_EXEC | O_SEARCH) # undef O_ACCMODE # define O_ACCMODE (O_RDONLY | O_WRONLY | O_RDWR | O_EXEC | O_SEARCH) #endif /* For systems that distinguish between text and binary I/O. O_BINARY is usually declared in fcntl.h */ #if !defined O_BINARY && defined _O_BINARY /* For MSC-compatible compilers. */ # define O_BINARY _O_BINARY # define O_TEXT _O_TEXT #endif #if defined __BEOS__ || defined __HAIKU__ /* BeOS 5 and Haiku have O_BINARY and O_TEXT, but they have no effect. */ # undef O_BINARY # undef O_TEXT #endif #ifndef O_BINARY # define O_BINARY 0 # define O_TEXT 0 #endif /* Fix up the AT_* macros. */ /* Work around a bug in Solaris 9 and 10: AT_FDCWD is positive. Its value exceeds INT_MAX, so its use as an int doesn't conform to the C standard, and GCC and Sun C complain in some cases. If the bug is present, undef AT_FDCWD here, so it can be redefined below. */ #if 0 < AT_FDCWD && AT_FDCWD == 0xffd19553 # undef AT_FDCWD #endif /* Use the same bit pattern as Solaris 9, but with the proper signedness. The bit pattern is important, in case this actually is Solaris with the above workaround. */ #ifndef AT_FDCWD # define AT_FDCWD (-3041965) #endif /* Use the same values as Solaris 9. This shouldn't matter, but there's no real reason to differ. */ #ifndef AT_SYMLINK_NOFOLLOW # define AT_SYMLINK_NOFOLLOW 4096 #endif #ifndef AT_REMOVEDIR # define AT_REMOVEDIR 1 #endif /* Solaris 9 lacks these two, so just pick unique values. */ #ifndef AT_SYMLINK_FOLLOW # define AT_SYMLINK_FOLLOW 2 #endif #ifndef AT_EACCESS # define AT_EACCESS 4 #endif #endif /* _@GUARD_PREFIX@_FCNTL_H */ #endif /* _@GUARD_PREFIX@_FCNTL_H */ #endif gnuastro-0.2.33-8a3b/bootstrapped/tests/ctype.in.h0000644000175000017500000000342113004436755016676 00000000000000/* A substitute for ISO C99 , for platforms on which it is incomplete. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible. */ /* * ISO C 99 for platforms on which it is incomplete. * */ #ifndef _@GUARD_PREFIX@_CTYPE_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* Include the original . */ /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_CTYPE_H@ #ifndef _@GUARD_PREFIX@_CTYPE_H #define _@GUARD_PREFIX@_CTYPE_H /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Return non-zero if c is a blank, i.e. a space or tab character. */ #if @GNULIB_ISBLANK@ # if !@HAVE_ISBLANK@ _GL_EXTERN_C int isblank (int c); # endif #elif defined GNULIB_POSIXCHECK # undef isblank # if HAVE_RAW_DECL_ISBLANK _GL_WARN_ON_USE (isblank, "isblank is unportable - " "use gnulib module isblank for portability"); # endif #endif #endif /* _@GUARD_PREFIX@_CTYPE_H */ #endif /* _@GUARD_PREFIX@_CTYPE_H */ gnuastro-0.2.33-8a3b/bootstrapped/tests/test-c-strcase.sh0000755000175000017500000000114313004436755020173 00000000000000#!/bin/sh # Test in the C locale. ./test-c-strcasecmp${EXEEXT} || exit 1 ./test-c-strncasecmp${EXEEXT} || exit 1 # Test in an ISO-8859-1 or ISO-8859-15 locale. : ${LOCALE_FR=fr_FR} if test $LOCALE_FR != none; then LC_ALL=$LOCALE_FR ./test-c-strcasecmp${EXEEXT} locale || exit 1 LC_ALL=$LOCALE_FR ./test-c-strncasecmp${EXEEXT} locale || exit 1 fi # Test in a Turkish UTF-8 locale. : ${LOCALE_TR_UTF8=tr_TR.UTF-8} if test $LOCALE_TR_UTF8 != none; then LC_ALL=$LOCALE_TR_UTF8 ./test-c-strcasecmp${EXEEXT} locale || exit 1 LC_ALL=$LOCALE_TR_UTF8 ./test-c-strncasecmp${EXEEXT} locale || exit 1 fi exit 0 gnuastro-0.2.33-8a3b/bootstrapped/tests/signature.h0000644000175000017500000000367613004436755017162 00000000000000/* Macro for checking that a function declaration is compliant. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef SIGNATURE_CHECK /* Check that the function FN takes the specified arguments ARGS with a return type of RET. This header is designed to be included after and the one system header that is supposed to contain the function being checked, but prior to any other system headers that are necessary for the unit test. Therefore, this file does not include any system headers, nor reference anything outside of the macro arguments. For an example, if foo.h should provide: extern int foo (char, float); then the unit test named test-foo.c would start out with: #include #include #include "signature.h" SIGNATURE_CHECK (foo, int, (char, float)); #include ... */ # define SIGNATURE_CHECK(fn, ret, args) \ SIGNATURE_CHECK1 (fn, ret, args, __LINE__) /* Necessary to allow multiple SIGNATURE_CHECK lines in a unit test. Note that the checks must not occupy the same line. */ # define SIGNATURE_CHECK1(fn, ret, args, id) \ SIGNATURE_CHECK2 (fn, ret, args, id) /* macroexpand line */ # define SIGNATURE_CHECK2(fn, ret, args, id) \ static ret (* _GL_UNUSED signature_check ## id) args = fn #endif /* SIGNATURE_CHECK */ gnuastro-0.2.33-8a3b/bootstrapped/tests/test-btowc2.sh0000755000175000017500000000056613004436755017517 00000000000000#!/bin/sh # Test whether a specific UTF-8 locale is installed. : ${LOCALE_FR_UTF8=fr_FR.UTF-8} if test $LOCALE_FR_UTF8 = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no french Unicode locale is installed" else echo "Skipping test: no french Unicode locale is supported" fi exit 77 fi LC_ALL=$LOCALE_FR_UTF8 \ ./test-btowc${EXEEXT} 2 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-btowc1.sh0000755000175000017500000000054313004436755017511 00000000000000#!/bin/sh # Test in an ISO-8859-1 or ISO-8859-15 locale. : ${LOCALE_FR=fr_FR} if test $LOCALE_FR = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no traditional french locale is installed" else echo "Skipping test: no traditional french locale is supported" fi exit 77 fi LC_ALL=$LOCALE_FR \ ./test-btowc${EXEEXT} 1 gnuastro-0.2.33-8a3b/bootstrapped/tests/macros.h0000644000175000017500000000650213004436755016434 00000000000000/* Common macros used by gnulib tests. Copyright (C) 2006-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* This file contains macros that are used by many gnulib tests. Put here only frequently used macros, say, used by 10 tests or more. */ #include #include /* Define ASSERT_STREAM before including this file if ASSERT must target a stream other than stderr. */ #ifndef ASSERT_STREAM # define ASSERT_STREAM stderr #endif /* ASSERT (condition); verifies that the specified condition is fulfilled. If not, a message is printed to ASSERT_STREAM if defined (defaulting to stderr if undefined) and the program is terminated with an error code. This macro has the following properties: - The programmer specifies the expected condition, not the failure condition. This simplifies thinking. - The condition is tested always, regardless of compilation flags. (Unlike the macro from .) - On Unix platforms, the tester can debug the test program with a debugger (provided core dumps are enabled: "ulimit -c unlimited"). - For the sake of platforms where no debugger is available (such as some mingw systems), an error message is printed on the error stream that includes the source location of the ASSERT invocation. */ #define ASSERT(expr) \ do \ { \ if (!(expr)) \ { \ fprintf (ASSERT_STREAM, "%s:%d: assertion '%s' failed\n", \ __FILE__, __LINE__, #expr); \ fflush (ASSERT_STREAM); \ abort (); \ } \ } \ while (0) /* SIZEOF (array) returns the number of elements of an array. It works for arrays that are declared outside functions and for local variables of array type. It does *not* work for function parameters of array type, because they are actually parameters of pointer type. */ #define SIZEOF(array) (sizeof (array) / sizeof (array[0])) /* STREQ (str1, str2) Return true if two strings compare equal. */ #define STREQ(a, b) (strcmp (a, b) == 0) /* Some numbers in the interval [0,1). */ extern const float randomf[1000]; extern const double randomd[1000]; extern const long double randoml[1000]; gnuastro-0.2.33-8a3b/bootstrapped/tests/test-binary-io.sh0000755000175000017500000000056313004436755020205 00000000000000#!/bin/sh tmpfiles="" trap 'rm -fr $tmpfiles' 1 2 3 15 tmpfiles="$tmpfiles t-bin-out0.tmp t-bin-out1.tmp t-bin-out2.tmp" ./test-binary-io${EXEEXT} 1 > t-bin-out1.tmp || exit 1 cmp t-bin-out0.tmp t-bin-out1.tmp > /dev/null || exit 1 ./test-binary-io${EXEEXT} 2 > t-bin-out2.tmp || exit 1 cmp t-bin-out0.tmp t-bin-out2.tmp > /dev/null || exit 1 rm -fr $tmpfiles exit 0 gnuastro-0.2.33-8a3b/bootstrapped/tests/test-argp-2.sh0000755000175000017500000000651313004436755017405 00000000000000#! /bin/sh # Test suite for argp. # Copyright (C) 2006-2016 Free Software Foundation, Inc. # This file is part of the GNUlib Library. # # This program is free software: you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see . */ TMP=argp.$$ unset ARGP_HELP_FMT ERR=0 func_compare() { # If argp was compiled without base_name, it will display full program name. # If run on mingw, it will display the program name with a .exe suffix. sed '1{ s,: [^ ]*/test-argp,: test-argp, s,: test-argp\.exe,: test-argp, }' | LC_ALL=C tr -d '\r' | diff -c $TMP - } #### # Test --usage output cat > $TMP < $TMP <$TMP <. EOT # Compare --help output, but filter out any bug-reporting email address. ./test-argp$EXEEXT --help \ | sed 's/^\(Report bugs to \)<[^>]*>.$/\1<>./' | func_compare || ERR=1 #### # Test ambiguous option handling ./test-argp$EXEEXT --optio 2>/dev/null && ERR=1 #### # Run built-in tests ./test-argp$EXEEXT || ERR=1 rm $TMP exit $ERR gnuastro-0.2.33-8a3b/bootstrapped/tests/test-wctype-h.c0000644000175000017500000000376513004436756017671 00000000000000/* Test of substitute. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "macros.h" /* Check that the type wint_t is defined. */ wint_t a = 'x'; /* Check that WEOF is defined. */ wint_t e = WEOF; /* Check that the type wctype_t is defined. */ wctype_t p; /* Check that the type wctrans_t is defined. */ wctrans_t q; int main (void) { /* Check that the isw* functions exist as functions or as macros. */ (void) iswalnum (0); (void) iswalpha (0); (void) iswcntrl (0); (void) iswdigit (0); (void) iswgraph (0); (void) iswlower (0); (void) iswprint (0); (void) iswpunct (0); (void) iswspace (0); (void) iswupper (0); (void) iswxdigit (0); /* Check that the isw* functions map WEOF to 0. */ ASSERT (!iswalnum (e)); ASSERT (!iswalpha (e)); ASSERT (!iswcntrl (e)); ASSERT (!iswdigit (e)); ASSERT (!iswgraph (e)); ASSERT (!iswlower (e)); ASSERT (!iswprint (e)); ASSERT (!iswpunct (e)); ASSERT (!iswspace (e)); ASSERT (!iswupper (e)); ASSERT (!iswxdigit (e)); /* Check that the tow* functions exist as functions or as macros. */ (void) towlower (0); (void) towupper (0); /* Check that the tow* functions map WEOF to WEOF. */ ASSERT (towlower (e) == e); ASSERT (towupper (e) == e); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-wcrtomb-w32.c0000644000175000017500000002171513004436756020212 00000000000000/* Test of conversion of wide character to multibyte character. Copyright (C) 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include #include #include #include #include "macros.h" #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ static int test_one_locale (const char *name, int codepage) { char buf[64]; size_t ret; # if 1 /* Portable code to set the locale. */ { char name_with_codepage[1024]; sprintf (name_with_codepage, "%s.%d", name, codepage); /* Set the locale. */ if (setlocale (LC_ALL, name_with_codepage) == NULL) return 77; } # else /* Hacky way to set a locale.codepage combination that setlocale() refuses to set. */ { /* Codepage of the current locale, set with setlocale(). Not necessarily the same as GetACP(). */ extern __declspec(dllimport) unsigned int __lc_codepage; /* Set the locale. */ if (setlocale (LC_ALL, name) == NULL) return 77; /* Clobber the codepage and MB_CUR_MAX, both set by setlocale(). */ __lc_codepage = codepage; switch (codepage) { case 1252: case 1256: MB_CUR_MAX = 1; break; case 932: case 950: case 936: MB_CUR_MAX = 2; break; case 54936: case 65001: MB_CUR_MAX = 4; break; } /* Test whether the codepage is really available. */ { mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, " ", 1, &state) == (size_t)(-1)) return 77; } } # endif /* Test NUL character. */ { buf[0] = 'x'; ret = wcrtomb (buf, 0, NULL); ASSERT (ret == 1); ASSERT (buf[0] == '\0'); } /* Test single bytes. */ { int c; for (c = 0; c < 0x100; c++) switch (c) { case '\t': case '\v': case '\f': case ' ': case '!': case '"': case '#': case '%': case '&': case '\'': case '(': case ')': case '*': case '+': case ',': case '-': case '.': case '/': case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': case ':': case ';': case '<': case '=': case '>': case '?': case 'A': case 'B': case 'C': case 'D': case 'E': case 'F': case 'G': case 'H': case 'I': case 'J': case 'K': case 'L': case 'M': case 'N': case 'O': case 'P': case 'Q': case 'R': case 'S': case 'T': case 'U': case 'V': case 'W': case 'X': case 'Y': case 'Z': case '[': case '\\': case ']': case '^': case '_': case 'a': case 'b': case 'c': case 'd': case 'e': case 'f': case 'g': case 'h': case 'i': case 'j': case 'k': case 'l': case 'm': case 'n': case 'o': case 'p': case 'q': case 'r': case 's': case 't': case 'u': case 'v': case 'w': case 'x': case 'y': case 'z': case '{': case '|': case '}': case '~': /* c is in the ISO C "basic character set". */ ret = wcrtomb (buf, btowc (c), NULL); ASSERT (ret == 1); ASSERT (buf[0] == (char) c); break; } } /* Test special calling convention, passing a NULL pointer. */ { ret = wcrtomb (NULL, '\0', NULL); ASSERT (ret == 1); ret = wcrtomb (NULL, btowc ('x'), NULL); ASSERT (ret == 1); } switch (codepage) { case 1252: /* Locale encoding is CP1252, an extension of ISO-8859-1. */ { /* Convert "B\374\337er": "Büßer" */ memset (buf, 'x', 8); ret = wcrtomb (buf, 0x00FC, NULL); ASSERT (ret == 1); ASSERT (memcmp (buf, "\374", 1) == 0); ASSERT (buf[1] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x00DF, NULL); ASSERT (ret == 1); ASSERT (memcmp (buf, "\337", 1) == 0); ASSERT (buf[1] == 'x'); } return 0; case 1256: /* Locale encoding is CP1256, not the same as ISO-8859-6. */ { /* Convert "x\302\341\346y": "xآلوy" */ memset (buf, 'x', 8); ret = wcrtomb (buf, 0x0622, NULL); ASSERT (ret == 1); ASSERT (memcmp (buf, "\302", 1) == 0); ASSERT (buf[1] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x0644, NULL); ASSERT (ret == 1); ASSERT (memcmp (buf, "\341", 1) == 0); ASSERT (buf[1] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x0648, NULL); ASSERT (ret == 1); ASSERT (memcmp (buf, "\346", 1) == 0); ASSERT (buf[1] == 'x'); } return 0; case 932: /* Locale encoding is CP932, similar to Shift_JIS. */ { /* Convert "<\223\372\226\173\214\352>": "<日本語>" */ memset (buf, 'x', 8); ret = wcrtomb (buf, 0x65E5, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\223\372", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x672C, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\226\173", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x8A9E, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\214\352", 2) == 0); ASSERT (buf[2] == 'x'); } return 0; case 950: /* Locale encoding is CP950, similar to Big5. */ { /* Convert "<\244\351\245\273\273\171>": "<日本語>" */ memset (buf, 'x', 8); ret = wcrtomb (buf, 0x65E5, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\244\351", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x672C, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\245\273", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x8A9E, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\273\171", 2) == 0); ASSERT (buf[2] == 'x'); } return 0; case 936: /* Locale encoding is CP936 = GBK, an extension of GB2312. */ { /* Convert "<\310\325\261\276\325\132>": "<日本語>" */ memset (buf, 'x', 8); ret = wcrtomb (buf, 0x65E5, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\310\325", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x672C, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\261\276", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x8A9E, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\325\132", 2) == 0); ASSERT (buf[2] == 'x'); } return 0; case 54936: /* Locale encoding is CP54936 = GB18030. */ { /* Convert "B\250\271\201\060\211\070er": "Büßer" */ memset (buf, 'x', 8); ret = wcrtomb (buf, 0x00FC, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\250\271", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x00DF, NULL); ASSERT (ret == 4); ASSERT (memcmp (buf, "\201\060\211\070", 4) == 0); ASSERT (buf[4] == 'x'); } return 0; case 65001: /* Locale encoding is CP65001 = UTF-8. */ { /* Convert "B\303\274\303\237er": "Büßer" */ memset (buf, 'x', 8); ret = wcrtomb (buf, 0x00FC, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\303\274", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x00DF, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\303\237", 2) == 0); ASSERT (buf[2] == 'x'); } return 0; default: return 1; } } int main (int argc, char *argv[]) { int codepage = atoi (argv[argc - 1]); int result; int i; result = 77; for (i = 1; i < argc - 1; i++) { int ret = test_one_locale (argv[i], codepage); if (ret != 77) result = ret; } if (result == 77) { fprintf (stderr, "Skipping test: found no locale with codepage %d\n", codepage); } return result; } #else int main (int argc, char *argv[]) { fputs ("Skipping test: not a native Windows system\n", stderr); return 77; } #endif gnuastro-0.2.33-8a3b/bootstrapped/tests/test-wcrtomb.c0000644000175000017500000001101613004436756017572 00000000000000/* Test of conversion of wide character to multibyte character. Copyright (C) 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include #include "signature.h" SIGNATURE_CHECK (wcrtomb, size_t, (char *, wchar_t, mbstate_t *)); #include #include #include #include "macros.h" /* Check the multibyte character s[0..n-1]. */ static void check_character (const char *s, size_t n) { wchar_t wc; char buf[64]; int iret; size_t ret; wc = (wchar_t) 0xBADFACE; iret = mbtowc (&wc, s, n); ASSERT (iret == n); ret = wcrtomb (buf, wc, NULL); ASSERT (ret == n); ASSERT (memcmp (buf, s, n) == 0); /* Test special calling convention, passing a NULL pointer. */ ret = wcrtomb (NULL, wc, NULL); ASSERT (ret == 1); } int main (int argc, char *argv[]) { char buf[64]; size_t ret; /* configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; /* Test NUL character. */ { buf[0] = 'x'; ret = wcrtomb (buf, 0, NULL); ASSERT (ret == 1); ASSERT (buf[0] == '\0'); } /* Test single bytes. */ { int c; for (c = 0; c < 0x100; c++) switch (c) { case '\t': case '\v': case '\f': case ' ': case '!': case '"': case '#': case '%': case '&': case '\'': case '(': case ')': case '*': case '+': case ',': case '-': case '.': case '/': case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': case ':': case ';': case '<': case '=': case '>': case '?': case 'A': case 'B': case 'C': case 'D': case 'E': case 'F': case 'G': case 'H': case 'I': case 'J': case 'K': case 'L': case 'M': case 'N': case 'O': case 'P': case 'Q': case 'R': case 'S': case 'T': case 'U': case 'V': case 'W': case 'X': case 'Y': case 'Z': case '[': case '\\': case ']': case '^': case '_': case 'a': case 'b': case 'c': case 'd': case 'e': case 'f': case 'g': case 'h': case 'i': case 'j': case 'k': case 'l': case 'm': case 'n': case 'o': case 'p': case 'q': case 'r': case 's': case 't': case 'u': case 'v': case 'w': case 'x': case 'y': case 'z': case '{': case '|': case '}': case '~': /* c is in the ISO C "basic character set". */ ret = wcrtomb (buf, btowc (c), NULL); ASSERT (ret == 1); ASSERT (buf[0] == (char) c); break; } } /* Test special calling convention, passing a NULL pointer. */ { ret = wcrtomb (NULL, '\0', NULL); ASSERT (ret == 1); ret = wcrtomb (NULL, btowc ('x'), NULL); ASSERT (ret == 1); } if (argc > 1) switch (argv[1][0]) { case '1': /* Locale encoding is ISO-8859-1 or ISO-8859-15. */ { const char input[] = "B\374\337er"; /* "Büßer" */ check_character (input + 1, 1); check_character (input + 2, 1); } return 0; case '2': /* Locale encoding is UTF-8. */ { const char input[] = "B\303\274\303\237er"; /* "Büßer" */ check_character (input + 1, 2); check_character (input + 3, 2); } return 0; case '3': /* Locale encoding is EUC-JP. */ { const char input[] = "<\306\374\313\334\270\354>"; /* "<日本語>" */ check_character (input + 1, 2); check_character (input + 3, 2); check_character (input + 5, 2); } return 0; case '4': /* Locale encoding is GB18030. */ { const char input[] = "B\250\271\201\060\211\070er"; /* "Büßer" */ check_character (input + 1, 2); check_character (input + 3, 4); } return 0; } return 1; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-wchar.c0000644000175000017500000000213513004436756017223 00000000000000/* Test of substitute. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" /* Check that the types wchar_t and wint_t are defined. */ wchar_t a = 'c'; wint_t b = 'x'; /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); int main (void) { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-vsnprintf.c0000644000175000017500000000430413004436756020150 00000000000000/* Test of vsnprintf() function. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "signature.h" SIGNATURE_CHECK (vsnprintf, int, (char *, size_t, char const *, va_list)); #include #include #include "macros.h" static int my_snprintf (char *buf, int size, const char *format, ...) { va_list args; int ret; va_start (args, format); ret = vsnprintf (buf, size, format, args); va_end (args); return ret; } int main (int argc, char *argv[]) { char buf[8]; int size; int retval; retval = my_snprintf (NULL, 0, "%d", 12345); ASSERT (retval == 5); for (size = 0; size <= 8; size++) { memcpy (buf, "DEADBEEF", 8); retval = my_snprintf (buf, size, "%d", 12345); ASSERT (retval == 5); if (size < 6) { if (size > 0) { ASSERT (memcmp (buf, "12345", size - 1) == 0); ASSERT (buf[size - 1] == '\0' || buf[size - 1] == '0' + size); } #if !CHECK_VSNPRINTF_POSIX if (size > 0) #endif ASSERT (memcmp (buf + size, &"DEADBEEF"[size], 8 - size) == 0); } else { ASSERT (memcmp (buf, "12345\0EF", 8) == 0); } } /* Test the support of the POSIX/XSI format strings with positions. */ { char result[100]; retval = my_snprintf (result, sizeof (result), "%2$d %1$d", 33, 55); ASSERT (strcmp (result, "55 33") == 0); ASSERT (retval == strlen (result)); } return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-verify.c0000644000175000017500000000350313004436756017423 00000000000000/* Test the "verify" module. Copyright (C) 2005, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible. */ #include #include "verify.h" #ifndef EXP_FAIL # define EXP_FAIL 0 #endif int x; enum { a, b, c }; #if EXP_FAIL == 1 verify (x >= 0); /* should give ERROR: non-constant expression */ #endif verify (c == 2); /* should be ok */ #if EXP_FAIL == 2 verify (1 + 1 == 3); /* should give ERROR */ #endif verify (1 == 1); verify (1 == 1); /* should be ok */ enum { item = verify_true (1 == 1) * 0 + 17 /* should be ok */ }; static int function (int n) { #if EXP_FAIL == 3 verify (n >= 0); /* should give ERROR: non-constant expression */ #endif verify (c == 2); /* should be ok */ #if EXP_FAIL == 4 verify (1 + 1 == 3); /* should give ERROR */ #endif verify (1 == 1); verify (1 == 1); /* should be ok */ if (n) return ((void) verify_expr (1 == 1, 1), verify_expr (1 == 1, 8)); /* should be ok */ #if EXP_FAIL == 5 return verify_expr (1 == 2, 5); /* should give ERROR */ #endif return 0; } int main (void) { return !(function (0) == 0 && function (1) == 8); } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-vasnprintf.c0000644000175000017500000000433513004436756020315 00000000000000/* Test of vasnprintf() and asnprintf() functions. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include "vasnprintf.h" #include #include #include #include "macros.h" static void test_function (char * (*my_asnprintf) (char *, size_t *, const char *, ...)) { char buf[8]; int size; for (size = 0; size <= 8; size++) { size_t length = size; char *result = my_asnprintf (NULL, &length, "%d", 12345); ASSERT (result != NULL); ASSERT (strcmp (result, "12345") == 0); ASSERT (length == 5); free (result); } for (size = 0; size <= 8; size++) { size_t length; char *result; memcpy (buf, "DEADBEEF", 8); length = size; result = my_asnprintf (buf, &length, "%d", 12345); ASSERT (result != NULL); ASSERT (strcmp (result, "12345") == 0); ASSERT (length == 5); if (size < 6) ASSERT (result != buf); ASSERT (memcmp (buf + size, &"DEADBEEF"[size], 8 - size) == 0); if (result != buf) free (result); } } static char * my_asnprintf (char *resultbuf, size_t *lengthp, const char *format, ...) { va_list args; char *ret; va_start (args, format); ret = vasnprintf (resultbuf, lengthp, format, args); va_end (args); return ret; } static void test_vasnprintf () { test_function (my_asnprintf); } static void test_asnprintf () { test_function (asnprintf); } int main (int argc, char *argv[]) { test_vasnprintf (); test_asnprintf (); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-unsetenv.c0000644000175000017500000000337513004436756017775 00000000000000/* Tests of unsetenv. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include #include "signature.h" SIGNATURE_CHECK (unsetenv, int, (char const *)); #include #include #include #include "macros.h" int main (void) { char entry[] = "b=2"; /* Test removal when multiple entries present. */ ASSERT (putenv ((char *) "a=1") == 0); ASSERT (putenv (entry) == 0); entry[0] = 'a'; /* Unspecified what getenv("a") would be at this point. */ ASSERT (unsetenv ("a") == 0); /* Both entries will be removed. */ ASSERT (getenv ("a") == NULL); ASSERT (unsetenv ("a") == 0); /* Required to fail with EINVAL. */ errno = 0; ASSERT (unsetenv ("") == -1); ASSERT (errno == EINVAL); errno = 0; ASSERT (unsetenv ("a=b") == -1); ASSERT (errno == EINVAL); #if 0 /* glibc and gnulib's implementation guarantee this, but POSIX no longer requires it: http://austingroupbugs.net/view.php?id=185 */ errno = 0; ASSERT (unsetenv (NULL) == -1); ASSERT (errno == EINVAL); #endif return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-unistd.c0000644000175000017500000000304713004436755017427 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); /* Check that the various SEEK_* macros are defined. */ int sk[] = { SEEK_CUR, SEEK_END, SEEK_SET }; /* Check that the various *_FILENO macros are defined. */ #if ! (defined STDIN_FILENO \ && (STDIN_FILENO + STDOUT_FILENO + STDERR_FILENO == 3)) missing or broken *_FILENO macros #endif /* Check that the types are all defined. */ size_t t1; ssize_t t2; #ifdef TODO /* Not implemented in gnulib yet */ uid_t t3; gid_t t4; #endif off_t t5; pid_t t6; #ifdef TODO useconds_t t7; intptr_t t8; #endif int main (void) { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-time.c0000644000175000017500000000236013004436755017054 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" /* Check that the types are all defined. */ struct timespec t1; #if 0 /* POSIX:2008 does not require pid_t in unconditionally, and indeed it's missing on Mac OS X 10.5, FreeBSD 6.4, OpenBSD 4.9, mingw. */ pid_t t2; #endif /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); int main (void) { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-thread_self.c0000644000175000017500000000215013004436755020373 00000000000000/* Test of gl_thread_self () macro. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2011. */ #include #include "glthread/thread.h" gl_thread_t main_thread; int main () { /* Check that gl_thread_self () can be used with just $(LIBTHREAD), not $(LIBMULTITHREAD), i.e. in libraries that are multithread-safe but don't create threads themselves. */ main_thread = gl_thread_self (); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-thread_create.c0000644000175000017500000000412313004436755020707 00000000000000/* Test of gl_thread_create () macro. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2011. */ #include #include "glthread/thread.h" #include #include #include "macros.h" static gl_thread_t main_thread_before; static gl_thread_t main_thread_after; static gl_thread_t worker_thread; static int dummy; static volatile int work_done; static void * worker_thread_func (void *arg) { work_done = 1; return &dummy; } int main () { main_thread_before = gl_thread_self (); if (glthread_create (&worker_thread, worker_thread_func, NULL) == 0) { void *ret; /* Check that gl_thread_self () has the same value before than after the first call to gl_thread_create (). */ main_thread_after = gl_thread_self (); ASSERT (memcmp (&main_thread_before, &main_thread_after, sizeof (gl_thread_t)) == 0); gl_thread_join (worker_thread, &ret); /* Check the return value of the thread. */ ASSERT (ret == &dummy); /* Check that worker_thread_func () has finished executing. */ ASSERT (work_done); return 0; } else { #if USE_POSIX_THREADS || USE_SOLARIS_THREADS || USE_PTH_THREADS || USE_WINDOWS_THREADS fputs ("glthread_create failed\n", stderr); return 1; #else fputs ("Skipping test: multithreading not enabled\n", stderr); return 77; #endif } } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-sysexits.c0000644000175000017500000000255113004436755020013 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include int exitcode; int main () { /* Check that all EX_* symbols are defined to integer constant expressions with mutually different values. */ switch (exitcode) { case EX_OK: case EX_USAGE: case EX_DATAERR: case EX_NOINPUT: case EX_NOUSER: case EX_NOHOST: case EX_UNAVAILABLE: case EX_SOFTWARE: case EX_OSERR: case EX_OSFILE: case EX_CANTCREAT: case EX_IOERR: case EX_TEMPFAIL: case EX_PROTOCOL: case EX_NOPERM: case EX_CONFIG: break; } return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-sys_types.c0000644000175000017500000000172113004436755020160 00000000000000/* Test of substitute. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2011. */ #include #include /* Check that the types are all defined. */ pid_t t1; size_t t2; ssize_t t3; off_t t4; mode_t t5; int main (void) { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-sys_time.c0000644000175000017500000000214713004436755017755 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include /* Check that the 'struct timeval' type is defined. */ struct timeval a; /* Check that a.tv_sec is wide enough to hold a time_t, ignoring signedness issues. */ typedef int verify_tv_sec_type[sizeof (time_t) <= sizeof (a.tv_sec) ? 1 : -1]; int main (void) { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-sys_stat.c0000644000175000017500000001626513004436755020000 00000000000000/* Test of substitute. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" /* Check the existence of some macros. */ int a[] = { S_IFMT, #ifdef S_IFBLK /* missing on MSVC */ S_IFBLK, #endif S_IFCHR, S_IFDIR, S_IFIFO, S_IFREG, #ifdef S_IFLNK /* missing on native Windows and DJGPP */ S_IFLNK, #endif #ifdef S_IFSOCK /* missing on native Windows and DJGPP */ S_IFSOCK, #endif S_IRWXU, S_IRUSR, S_IWUSR, S_IXUSR, S_IRWXG, S_IRGRP, S_IWGRP, S_IXGRP, S_IRWXO, S_IROTH, S_IWOTH, S_IXOTH, S_ISUID, S_ISGID, S_ISVTX, S_ISBLK (S_IFREG), S_ISCHR (S_IFREG), S_ISDIR (S_IFREG), S_ISFIFO (S_IFREG), S_ISREG (S_IFREG), S_ISLNK (S_IFREG), S_ISSOCK (S_IFREG), S_ISDOOR (S_IFREG), S_ISMPB (S_IFREG), S_ISMPX (S_IFREG), S_ISNAM (S_IFREG), S_ISNWK (S_IFREG), S_ISPORT (S_IFREG), S_ISCTG (S_IFREG), S_ISOFD (S_IFREG), S_ISOFL (S_IFREG), S_ISWHT (S_IFREG) }; /* Sanity checks. */ verify (S_IRWXU == (S_IRUSR | S_IWUSR | S_IXUSR)); verify (S_IRWXG == (S_IRGRP | S_IWGRP | S_IXGRP)); verify (S_IRWXO == (S_IROTH | S_IWOTH | S_IXOTH)); #ifdef S_IFBLK verify (S_ISBLK (S_IFBLK)); #endif verify (!S_ISBLK (S_IFCHR)); verify (!S_ISBLK (S_IFDIR)); verify (!S_ISBLK (S_IFIFO)); verify (!S_ISBLK (S_IFREG)); #ifdef S_IFLNK verify (!S_ISBLK (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISBLK (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISCHR (S_IFBLK)); #endif verify (S_ISCHR (S_IFCHR)); verify (!S_ISCHR (S_IFDIR)); verify (!S_ISCHR (S_IFIFO)); verify (!S_ISCHR (S_IFREG)); #ifdef S_IFLNK verify (!S_ISCHR (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISCHR (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISDIR (S_IFBLK)); #endif verify (!S_ISDIR (S_IFCHR)); verify (S_ISDIR (S_IFDIR)); verify (!S_ISDIR (S_IFIFO)); verify (!S_ISDIR (S_IFREG)); #ifdef S_IFLNK verify (!S_ISDIR (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISDIR (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISFIFO (S_IFBLK)); #endif verify (!S_ISFIFO (S_IFCHR)); verify (!S_ISFIFO (S_IFDIR)); verify (S_ISFIFO (S_IFIFO)); verify (!S_ISFIFO (S_IFREG)); #ifdef S_IFLNK verify (!S_ISFIFO (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISFIFO (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISREG (S_IFBLK)); #endif verify (!S_ISREG (S_IFCHR)); verify (!S_ISREG (S_IFDIR)); verify (!S_ISREG (S_IFIFO)); verify (S_ISREG (S_IFREG)); #ifdef S_IFLNK verify (!S_ISREG (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISREG (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISLNK (S_IFBLK)); #endif verify (!S_ISLNK (S_IFCHR)); verify (!S_ISLNK (S_IFDIR)); verify (!S_ISLNK (S_IFIFO)); verify (!S_ISLNK (S_IFREG)); #ifdef S_IFLNK verify (S_ISLNK (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISLNK (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISSOCK (S_IFBLK)); #endif verify (!S_ISSOCK (S_IFCHR)); verify (!S_ISSOCK (S_IFDIR)); verify (!S_ISSOCK (S_IFIFO)); verify (!S_ISSOCK (S_IFREG)); #ifdef S_IFLNK verify (!S_ISSOCK (S_IFLNK)); #endif #ifdef S_IFSOCK verify (S_ISSOCK (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISDOOR (S_IFBLK)); #endif verify (!S_ISDOOR (S_IFCHR)); verify (!S_ISDOOR (S_IFDIR)); verify (!S_ISDOOR (S_IFIFO)); verify (!S_ISDOOR (S_IFREG)); #ifdef S_IFLNK verify (!S_ISDOOR (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISDOOR (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISMPB (S_IFBLK)); #endif verify (!S_ISMPB (S_IFCHR)); verify (!S_ISMPB (S_IFDIR)); verify (!S_ISMPB (S_IFIFO)); verify (!S_ISMPB (S_IFREG)); #ifdef S_IFLNK verify (!S_ISMPB (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISMPB (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISMPX (S_IFBLK)); #endif verify (!S_ISMPX (S_IFCHR)); verify (!S_ISMPX (S_IFDIR)); verify (!S_ISMPX (S_IFIFO)); verify (!S_ISMPX (S_IFREG)); #ifdef S_IFLNK verify (!S_ISMPX (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISMPX (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISNAM (S_IFBLK)); #endif verify (!S_ISNAM (S_IFCHR)); verify (!S_ISNAM (S_IFDIR)); verify (!S_ISNAM (S_IFIFO)); verify (!S_ISNAM (S_IFREG)); #ifdef S_IFLNK verify (!S_ISNAM (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISNAM (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISNWK (S_IFBLK)); #endif verify (!S_ISNWK (S_IFCHR)); verify (!S_ISNWK (S_IFDIR)); verify (!S_ISNWK (S_IFIFO)); verify (!S_ISNWK (S_IFREG)); #ifdef S_IFLNK verify (!S_ISNWK (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISNWK (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISPORT (S_IFBLK)); #endif verify (!S_ISPORT (S_IFCHR)); verify (!S_ISPORT (S_IFDIR)); verify (!S_ISPORT (S_IFIFO)); verify (!S_ISPORT (S_IFREG)); #ifdef S_IFLNK verify (!S_ISPORT (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISPORT (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISCTG (S_IFBLK)); #endif verify (!S_ISCTG (S_IFCHR)); verify (!S_ISCTG (S_IFDIR)); verify (!S_ISCTG (S_IFIFO)); verify (!S_ISCTG (S_IFREG)); #ifdef S_IFLNK verify (!S_ISCTG (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISCTG (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISOFD (S_IFBLK)); #endif verify (!S_ISOFD (S_IFCHR)); verify (!S_ISOFD (S_IFDIR)); verify (!S_ISOFD (S_IFIFO)); verify (!S_ISOFD (S_IFREG)); #ifdef S_IFLNK verify (!S_ISOFD (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISOFD (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISOFL (S_IFBLK)); #endif verify (!S_ISOFL (S_IFCHR)); verify (!S_ISOFL (S_IFDIR)); verify (!S_ISOFL (S_IFIFO)); verify (!S_ISOFL (S_IFREG)); #ifdef S_IFLNK verify (!S_ISOFL (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISOFL (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISWHT (S_IFBLK)); #endif verify (!S_ISWHT (S_IFCHR)); verify (!S_ISWHT (S_IFDIR)); verify (!S_ISWHT (S_IFIFO)); verify (!S_ISWHT (S_IFREG)); #ifdef S_IFLNK verify (!S_ISWHT (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISWHT (S_IFSOCK)); #endif /* POSIX 2008 requires traditional encoding of permission constants. */ verify (S_IRWXU == 00700); verify (S_IRUSR == 00400); verify (S_IWUSR == 00200); verify (S_IXUSR == 00100); verify (S_IRWXG == 00070); verify (S_IRGRP == 00040); verify (S_IWGRP == 00020); verify (S_IXGRP == 00010); verify (S_IRWXO == 00007); verify (S_IROTH == 00004); verify (S_IWOTH == 00002); verify (S_IXOTH == 00001); verify (S_ISUID == 04000); verify (S_ISGID == 02000); verify (S_ISVTX == 01000); #if ((0 <= UTIME_NOW && UTIME_NOW < 1000000000) \ || (0 <= UTIME_OMIT && UTIME_OMIT < 1000000000) \ || UTIME_NOW == UTIME_OMIT) invalid UTIME macros #endif /* Check the existence of some types. */ nlink_t t1; off_t t2; mode_t t3; struct timespec st; int main (void) { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-symlink.c0000644000175000017500000000242213004436755017603 00000000000000/* Tests of symlink. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include #include "signature.h" SIGNATURE_CHECK (symlink, int, (char const *, char const *)); #include #include #include #include #include #include #include "ignore-value.h" #include "macros.h" #define BASE "test-symlink.t" #include "test-symlink.h" int main (void) { /* Remove any leftovers from a previous partial run. */ ignore_value (system ("rm -rf " BASE "*")); return test_symlink (symlink, true); } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-strnlen.c0000644000175000017500000000336113004436755017605 00000000000000/* * Copyright (C) 2010-2016 Free Software Foundation, Inc. * Written by Eric Blake * * This program is free software: you can redistribute it and/or modify * it under the terms of the GNU General Public License as published by * the Free Software Foundation; either version 3 of the License, or * (at your option) any later version. * * This program is distributed in the hope that it will be useful, * but WITHOUT ANY WARRANTY; without even the implied warranty of * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * GNU General Public License for more details. * * You should have received a copy of the GNU General Public License * along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (strnlen, size_t, (char const *, size_t)); #include #include "zerosize-ptr.h" #include "macros.h" int main (void) { size_t i; char *page_boundary = (char *) zerosize_ptr (); if (!page_boundary) { page_boundary = malloc (0x1000); ASSERT (page_boundary); page_boundary += 0x1000; } /* Basic behavior tests. */ ASSERT (strnlen ("a", 0) == 0); ASSERT (strnlen ("a", 1) == 1); ASSERT (strnlen ("a", 2) == 1); ASSERT (strnlen ("", 0x100000) == 0); /* Memory fence and alignment testing. */ for (i = 0; i < 512; i++) { char *start = page_boundary - i; size_t j = i; memset (start, 'x', i); do { if (i != j) { start[j] = 0; ASSERT (strnlen (start, i + j) == j); } ASSERT (strnlen (start, i) == j); ASSERT (strnlen (start, j) == j); } while (j--); } return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-strings.c0000644000175000017500000000155313004436755017612 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include int main () { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-string.c0000644000175000017500000000200713004436755017422 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); int main (void) { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-strerror.c0000644000175000017500000000370713004436755020006 00000000000000/* Test of strerror() function. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Eric Blake , 2007. */ #include #include #include "signature.h" SIGNATURE_CHECK (strerror, char *, (int)); #include #include "macros.h" int main (void) { char *str; errno = 0; str = strerror (EACCES); ASSERT (str); ASSERT (*str); ASSERT (errno == 0); errno = 0; str = strerror (ETIMEDOUT); ASSERT (str); ASSERT (*str); ASSERT (errno == 0); errno = 0; str = strerror (EOVERFLOW); ASSERT (str); ASSERT (*str); ASSERT (errno == 0); /* POSIX requires strerror (0) to succeed. Reject use of "Unknown error", but allow "Success", "No error", or even Solaris' "Error 0" which are distinct patterns from true out-of-range strings. http://austingroupbugs.net/view.php?id=382 */ errno = 0; str = strerror (0); ASSERT (str); ASSERT (*str); ASSERT (errno == 0); ASSERT (strstr (str, "nknown") == NULL); ASSERT (strstr (str, "ndefined") == NULL); /* POSIX requires strerror to produce a non-NULL result for all inputs; as an extension, we also guarantee a non-empty result. Reporting EINVAL is optional. */ errno = 0; str = strerror (-3); ASSERT (str); ASSERT (*str); ASSERT (errno == 0 || errno == EINVAL); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-strchrnul.c0000644000175000017500000000444613004436755020151 00000000000000/* * Copyright (C) 2008-2016 Free Software Foundation, Inc. * Written by Eric Blake and Bruno Haible * * This program is free software: you can redistribute it and/or modify * it under the terms of the GNU General Public License as published by * the Free Software Foundation; either version 3 of the License, or * (at your option) any later version. * * This program is distributed in the hope that it will be useful, * but WITHOUT ANY WARRANTY; without even the implied warranty of * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * GNU General Public License for more details. * * You should have received a copy of the GNU General Public License * along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (strchrnul, char *, (char const *, int)); #include #include "macros.h" int main (void) { size_t n = 0x100000; char *input = malloc (n + 1); ASSERT (input); input[0] = 'a'; input[1] = 'b'; memset (input + 2, 'c', 1024); memset (input + 1026, 'd', n - 1028); input[n - 2] = 'e'; input[n - 1] = 'a'; input[n] = '\0'; /* Basic behavior tests. */ ASSERT (strchrnul (input, 'a') == input); ASSERT (strchrnul (input, 'b') == input + 1); ASSERT (strchrnul (input, 'c') == input + 2); ASSERT (strchrnul (input, 'd') == input + 1026); ASSERT (strchrnul (input + 1, 'a') == input + n - 1); ASSERT (strchrnul (input + 1, 'e') == input + n - 2); ASSERT (strchrnul (input, 'f') == input + n); ASSERT (strchrnul (input, '\0') == input + n); /* Check that a very long haystack is handled quickly if the byte is found near the beginning. */ { size_t repeat = 10000; for (; repeat > 0; repeat--) { ASSERT (strchrnul (input, 'c') == input + 2); } } /* Alignment tests. */ { int i, j; for (i = 0; i < 32; i++) { for (j = 0; j < 256; j++) input[i + j] = (j + 1) & 0xff; for (j = 1; j < 256; j++) { ASSERT (strchrnul (input + i, j) == input + i + j - 1); input[i + j - 1] = (j == 1 ? 2 : 1); ASSERT (strchrnul (input + i, j) == input + i + 255); input[i + j - 1] = j; } } } free (input); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-stdlib.c0000644000175000017500000000262413004436755017402 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" /* Check that EXIT_SUCCESS is 0, per POSIX. */ static int exitcode = EXIT_SUCCESS; #if EXIT_SUCCESS "oops" #endif /* Check for GNU value (not guaranteed by POSIX, but is guaranteed by gnulib). */ #if EXIT_FAILURE != 1 "oops" #endif /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); #if GNULIB_TEST_SYSTEM_POSIX # include "test-sys_wait.h" #else # define test_sys_wait_macros() 0 #endif int main (void) { if (test_sys_wait_macros ()) return 1; return exitcode; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-stdio.c0000644000175000017500000000232213004436755017236 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" /* Check that the various SEEK_* macros are defined. */ int sk[] = { SEEK_CUR, SEEK_END, SEEK_SET }; /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); /* Check that the types are all defined. */ fpos_t t1; off_t t2; size_t t3; ssize_t t4; va_list t5; int main (void) { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-stdint.c0000644000175000017500000003330513004436755017426 00000000000000/* Test of substitute. Copyright (C) 2006-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2006. */ #include /* Whether to enable pedantic checks. */ #define DO_PEDANTIC 0 #include #include "verify.h" #include "intprops.h" #if __GNUC__ >= 2 && DO_PEDANTIC # define verify_same_types(expr1,expr2) \ extern void _verify_func(__LINE__) (__typeof__ (expr1) *); \ extern void _verify_func(__LINE__) (__typeof__ (expr2) *); # define _verify_func(line) _verify_func2(line) # define _verify_func2(line) verify_func_ ## line #else # define verify_same_types(expr1,expr2) extern void verify_func (int) #endif /* 7.18.1.1. Exact-width integer types */ /* 7.18.2.1. Limits of exact-width integer types */ int8_t a1[3] = { INT8_C (17), INT8_MIN, INT8_MAX }; verify (TYPE_MINIMUM (int8_t) == INT8_MIN); verify (TYPE_MAXIMUM (int8_t) == INT8_MAX); verify_same_types (INT8_MIN, (int8_t) 0 + 0); verify_same_types (INT8_MAX, (int8_t) 0 + 0); int16_t a2[3] = { INT16_C (17), INT16_MIN, INT16_MAX }; verify (TYPE_MINIMUM (int16_t) == INT16_MIN); verify (TYPE_MAXIMUM (int16_t) == INT16_MAX); verify_same_types (INT16_MIN, (int16_t) 0 + 0); verify_same_types (INT16_MAX, (int16_t) 0 + 0); int32_t a3[3] = { INT32_C (17), INT32_MIN, INT32_MAX }; verify (TYPE_MINIMUM (int32_t) == INT32_MIN); verify (TYPE_MAXIMUM (int32_t) == INT32_MAX); verify_same_types (INT32_MIN, (int32_t) 0 + 0); verify_same_types (INT32_MAX, (int32_t) 0 + 0); #ifdef INT64_MAX int64_t a4[3] = { INT64_C (17), INT64_MIN, INT64_MAX }; verify (TYPE_MINIMUM (int64_t) == INT64_MIN); verify (TYPE_MAXIMUM (int64_t) == INT64_MAX); verify_same_types (INT64_MIN, (int64_t) 0 + 0); verify_same_types (INT64_MAX, (int64_t) 0 + 0); #endif uint8_t b1[2] = { UINT8_C (17), UINT8_MAX }; verify (TYPE_MAXIMUM (uint8_t) == UINT8_MAX); verify_same_types (UINT8_MAX, (uint8_t) 0 + 0); uint16_t b2[2] = { UINT16_C (17), UINT16_MAX }; verify (TYPE_MAXIMUM (uint16_t) == UINT16_MAX); verify_same_types (UINT16_MAX, (uint16_t) 0 + 0); uint32_t b3[2] = { UINT32_C (17), UINT32_MAX }; verify (TYPE_MAXIMUM (uint32_t) == UINT32_MAX); verify_same_types (UINT32_MAX, (uint32_t) 0 + 0); #ifdef UINT64_MAX uint64_t b4[2] = { UINT64_C (17), UINT64_MAX }; verify (TYPE_MAXIMUM (uint64_t) == UINT64_MAX); verify_same_types (UINT64_MAX, (uint64_t) 0 + 0); #endif #if INT8_MIN && INT8_MAX && INT16_MIN && INT16_MAX && INT32_MIN && INT32_MAX /* ok */ #else err or; #endif #if UINT8_MAX && UINT16_MAX && UINT32_MAX /* ok */ #else err or; #endif /* 7.18.1.2. Minimum-width integer types */ /* 7.18.2.2. Limits of minimum-width integer types */ int_least8_t c1[3] = { 17, INT_LEAST8_MIN, INT_LEAST8_MAX }; verify (TYPE_MINIMUM (int_least8_t) == INT_LEAST8_MIN); verify (TYPE_MAXIMUM (int_least8_t) == INT_LEAST8_MAX); verify_same_types (INT_LEAST8_MIN, (int_least8_t) 0 + 0); verify_same_types (INT_LEAST8_MAX, (int_least8_t) 0 + 0); int_least16_t c2[3] = { 17, INT_LEAST16_MIN, INT_LEAST16_MAX }; verify (TYPE_MINIMUM (int_least16_t) == INT_LEAST16_MIN); verify (TYPE_MAXIMUM (int_least16_t) == INT_LEAST16_MAX); verify_same_types (INT_LEAST16_MIN, (int_least16_t) 0 + 0); verify_same_types (INT_LEAST16_MAX, (int_least16_t) 0 + 0); int_least32_t c3[3] = { 17, INT_LEAST32_MIN, INT_LEAST32_MAX }; verify (TYPE_MINIMUM (int_least32_t) == INT_LEAST32_MIN); verify (TYPE_MAXIMUM (int_least32_t) == INT_LEAST32_MAX); verify_same_types (INT_LEAST32_MIN, (int_least32_t) 0 + 0); verify_same_types (INT_LEAST32_MAX, (int_least32_t) 0 + 0); #ifdef INT_LEAST64_MAX int_least64_t c4[3] = { 17, INT_LEAST64_MIN, INT_LEAST64_MAX }; verify (TYPE_MINIMUM (int_least64_t) == INT_LEAST64_MIN); verify (TYPE_MAXIMUM (int_least64_t) == INT_LEAST64_MAX); verify_same_types (INT_LEAST64_MIN, (int_least64_t) 0 + 0); verify_same_types (INT_LEAST64_MAX, (int_least64_t) 0 + 0); #endif uint_least8_t d1[2] = { 17, UINT_LEAST8_MAX }; verify (TYPE_MAXIMUM (uint_least8_t) == UINT_LEAST8_MAX); verify_same_types (UINT_LEAST8_MAX, (uint_least8_t) 0 + 0); uint_least16_t d2[2] = { 17, UINT_LEAST16_MAX }; verify (TYPE_MAXIMUM (uint_least16_t) == UINT_LEAST16_MAX); verify_same_types (UINT_LEAST16_MAX, (uint_least16_t) 0 + 0); uint_least32_t d3[2] = { 17, UINT_LEAST32_MAX }; verify (TYPE_MAXIMUM (uint_least32_t) == UINT_LEAST32_MAX); verify_same_types (UINT_LEAST32_MAX, (uint_least32_t) 0 + 0); #ifdef UINT_LEAST64_MAX uint_least64_t d4[2] = { 17, UINT_LEAST64_MAX }; verify (TYPE_MAXIMUM (uint_least64_t) == UINT_LEAST64_MAX); verify_same_types (UINT_LEAST64_MAX, (uint_least64_t) 0 + 0); #endif #if INT_LEAST8_MIN && INT_LEAST8_MAX && INT_LEAST16_MIN && INT_LEAST16_MAX && INT_LEAST32_MIN && INT_LEAST32_MAX /* ok */ #else err or; #endif #if UINT_LEAST8_MAX && UINT_LEAST16_MAX && UINT_LEAST32_MAX /* ok */ #else err or; #endif /* 7.18.1.3. Fastest minimum-width integer types */ /* 7.18.2.3. Limits of fastest minimum-width integer types */ int_fast8_t e1[3] = { 17, INT_FAST8_MIN, INT_FAST8_MAX }; verify (TYPE_MINIMUM (int_fast8_t) == INT_FAST8_MIN); verify (TYPE_MAXIMUM (int_fast8_t) == INT_FAST8_MAX); verify_same_types (INT_FAST8_MIN, (int_fast8_t) 0 + 0); verify_same_types (INT_FAST8_MAX, (int_fast8_t) 0 + 0); int_fast16_t e2[3] = { 17, INT_FAST16_MIN, INT_FAST16_MAX }; verify (TYPE_MINIMUM (int_fast16_t) == INT_FAST16_MIN); verify (TYPE_MAXIMUM (int_fast16_t) == INT_FAST16_MAX); verify_same_types (INT_FAST16_MIN, (int_fast16_t) 0 + 0); verify_same_types (INT_FAST16_MAX, (int_fast16_t) 0 + 0); int_fast32_t e3[3] = { 17, INT_FAST32_MIN, INT_FAST32_MAX }; verify (TYPE_MINIMUM (int_fast32_t) == INT_FAST32_MIN); verify (TYPE_MAXIMUM (int_fast32_t) == INT_FAST32_MAX); verify_same_types (INT_FAST32_MIN, (int_fast32_t) 0 + 0); verify_same_types (INT_FAST32_MAX, (int_fast32_t) 0 + 0); #ifdef INT_FAST64_MAX int_fast64_t e4[3] = { 17, INT_FAST64_MIN, INT_FAST64_MAX }; verify (TYPE_MINIMUM (int_fast64_t) == INT_FAST64_MIN); verify (TYPE_MAXIMUM (int_fast64_t) == INT_FAST64_MAX); verify_same_types (INT_FAST64_MIN, (int_fast64_t) 0 + 0); verify_same_types (INT_FAST64_MAX, (int_fast64_t) 0 + 0); #endif uint_fast8_t f1[2] = { 17, UINT_FAST8_MAX }; verify (TYPE_MAXIMUM (uint_fast8_t) == UINT_FAST8_MAX); verify_same_types (UINT_FAST8_MAX, (uint_fast8_t) 0 + 0); uint_fast16_t f2[2] = { 17, UINT_FAST16_MAX }; verify (TYPE_MAXIMUM (uint_fast16_t) == UINT_FAST16_MAX); verify_same_types (UINT_FAST16_MAX, (uint_fast16_t) 0 + 0); uint_fast32_t f3[2] = { 17, UINT_FAST32_MAX }; verify (TYPE_MAXIMUM (uint_fast32_t) == UINT_FAST32_MAX); verify_same_types (UINT_FAST32_MAX, (uint_fast32_t) 0 + 0); #ifdef UINT_FAST64_MAX uint_fast64_t f4[2] = { 17, UINT_FAST64_MAX }; verify (TYPE_MAXIMUM (uint_fast64_t) == UINT_FAST64_MAX); verify_same_types (UINT_FAST64_MAX, (uint_fast64_t) 0 + 0); #endif #if INT_FAST8_MIN && INT_FAST8_MAX && INT_FAST16_MIN && INT_FAST16_MAX && INT_FAST32_MIN && INT_FAST32_MAX /* ok */ #else err or; #endif #if UINT_FAST8_MAX && UINT_FAST16_MAX && UINT_FAST32_MAX /* ok */ #else err or; #endif /* 7.18.1.4. Integer types capable of holding object pointers */ /* 7.18.2.4. Limits of integer types capable of holding object pointers */ intptr_t g[3] = { 17, INTPTR_MIN, INTPTR_MAX }; verify (TYPE_MINIMUM (intptr_t) == INTPTR_MIN); verify (TYPE_MAXIMUM (intptr_t) == INTPTR_MAX); verify_same_types (INTPTR_MIN, (intptr_t) 0 + 0); verify_same_types (INTPTR_MAX, (intptr_t) 0 + 0); uintptr_t h[2] = { 17, UINTPTR_MAX }; verify (TYPE_MAXIMUM (uintptr_t) == UINTPTR_MAX); verify_same_types (UINTPTR_MAX, (uintptr_t) 0 + 0); #if INTPTR_MIN && INTPTR_MAX && UINTPTR_MAX /* ok */ #else err or; #endif /* 7.18.1.5. Greatest-width integer types */ /* 7.18.2.5. Limits of greatest-width integer types */ intmax_t i[3] = { INTMAX_C (17), INTMAX_MIN, INTMAX_MAX }; verify (TYPE_MINIMUM (intmax_t) == INTMAX_MIN); verify (TYPE_MAXIMUM (intmax_t) == INTMAX_MAX); verify_same_types (INTMAX_MIN, (intmax_t) 0 + 0); verify_same_types (INTMAX_MAX, (intmax_t) 0 + 0); uintmax_t j[2] = { UINTMAX_C (17), UINTMAX_MAX }; verify (TYPE_MAXIMUM (uintmax_t) == UINTMAX_MAX); verify_same_types (UINTMAX_MAX, (uintmax_t) 0 + 0); /* As of 2007, Sun C and HP-UX 10.20 cc don't support 'long long' constants in the preprocessor. */ #if !(defined __SUNPRO_C || (defined __hpux && !defined __GNUC__)) #if INTMAX_MIN && INTMAX_MAX && UINTMAX_MAX /* ok */ #else err or; #endif #endif /* 7.18.3. Limits of other integer types */ #include verify (TYPE_MINIMUM (ptrdiff_t) == PTRDIFF_MIN); verify (TYPE_MAXIMUM (ptrdiff_t) == PTRDIFF_MAX); verify_same_types (PTRDIFF_MIN, (ptrdiff_t) 0 + 0); verify_same_types (PTRDIFF_MAX, (ptrdiff_t) 0 + 0); #if PTRDIFF_MIN && PTRDIFF_MAX /* ok */ #else err or; #endif #include verify (TYPE_MINIMUM (sig_atomic_t) == SIG_ATOMIC_MIN); verify (TYPE_MAXIMUM (sig_atomic_t) == SIG_ATOMIC_MAX); verify_same_types (SIG_ATOMIC_MIN, (sig_atomic_t) 0 + 0); verify_same_types (SIG_ATOMIC_MAX, (sig_atomic_t) 0 + 0); #if SIG_ATOMIC_MIN != 17 && SIG_ATOMIC_MAX /* ok */ #else err or; #endif verify (TYPE_MAXIMUM (size_t) == SIZE_MAX); verify_same_types (SIZE_MAX, (size_t) 0 + 0); #if SIZE_MAX /* ok */ #else err or; #endif #if HAVE_WCHAR_T verify (TYPE_MINIMUM (wchar_t) == WCHAR_MIN); verify (TYPE_MAXIMUM (wchar_t) == WCHAR_MAX); verify_same_types (WCHAR_MIN, (wchar_t) 0 + 0); verify_same_types (WCHAR_MAX, (wchar_t) 0 + 0); # if WCHAR_MIN != 17 && WCHAR_MAX /* ok */ # else err or; # endif #endif #if HAVE_WINT_T # include verify (TYPE_MINIMUM (wint_t) == WINT_MIN); verify (TYPE_MAXIMUM (wint_t) == WINT_MAX); verify_same_types (WINT_MIN, (wint_t) 0 + 0); verify_same_types (WINT_MAX, (wint_t) 0 + 0); # if WINT_MIN != 17 && WINT_MAX /* ok */ # else err or; # endif #endif /* 7.18.4. Macros for integer constants */ verify (INT8_C (17) == 17); verify_same_types (INT8_C (17), (int_least8_t)0 + 0); verify (UINT8_C (17) == 17); verify_same_types (UINT8_C (17), (uint_least8_t)0 + 0); verify (INT16_C (17) == 17); verify_same_types (INT16_C (17), (int_least16_t)0 + 0); verify (UINT16_C (17) == 17); verify_same_types (UINT16_C (17), (uint_least16_t)0 + 0); verify (INT32_C (17) == 17); verify_same_types (INT32_C (17), (int_least32_t)0 + 0); verify (UINT32_C (17) == 17); verify_same_types (UINT32_C (17), (uint_least32_t)0 + 0); #ifdef INT64_C verify (INT64_C (17) == 17); verify_same_types (INT64_C (17), (int_least64_t)0 + 0); #endif #ifdef UINT64_C verify (UINT64_C (17) == 17); verify_same_types (UINT64_C (17), (uint_least64_t)0 + 0); #endif verify (INTMAX_C (17) == 17); verify_same_types (INTMAX_C (17), (intmax_t)0 + 0); verify (UINTMAX_C (17) == 17); verify_same_types (UINTMAX_C (17), (uintmax_t)0 + 0); /* Use _GL_VERIFY (with a fixed-length diagnostic string) rather than verify, because the latter would require forming each stringified expression, and many of these would be so long as to trigger a warning/error like this: test-stdint.c:407:1: error: string length '6980' is greater than the \ length '4095' ISO C99 compilers are required to support \ [-Werror=overlength-strings] */ #define verify_width(width, min, max) \ _GL_VERIFY ((max) >> ((width) - 1 - ((min) < 0)) == 1, \ "verify_width check") /* Macros specified by ISO/IEC TS 18661-1:2014. */ #ifdef INT8_MAX verify_width (INT8_WIDTH, INT8_MIN, INT8_MAX); #endif #ifdef UINT8_MAX verify_width (UINT8_WIDTH, 0, UINT8_MAX); #endif #ifdef INT16_MAX verify_width (INT16_WIDTH, INT16_MIN, INT16_MAX); #endif #ifdef UINT16_MAX verify_width (UINT16_WIDTH, 0, UINT16_MAX); #endif #ifdef INT32_MAX verify_width (INT32_WIDTH, INT32_MIN, INT32_MAX); #endif #ifdef UINT32_MAX verify_width (UINT32_WIDTH, 0, UINT32_MAX); #endif #ifdef INT64_MAX verify_width (INT64_WIDTH, INT64_MIN, INT64_MAX); #endif #ifdef UINT64_MAX verify_width (UINT64_WIDTH, 0, UINT64_MAX); #endif verify_width (INT_LEAST8_WIDTH, INT_LEAST8_MIN, INT_LEAST8_MAX); verify_width (UINT_LEAST8_WIDTH, 0, UINT_LEAST8_MAX); verify_width (INT_LEAST16_WIDTH, INT_LEAST16_MIN, INT_LEAST16_MAX); verify_width (UINT_LEAST16_WIDTH, 0, UINT_LEAST16_MAX); verify_width (INT_LEAST32_WIDTH, INT_LEAST32_MIN, INT_LEAST32_MAX); verify_width (UINT_LEAST32_WIDTH, 0, UINT_LEAST32_MAX); verify_width (INT_LEAST64_WIDTH, INT_LEAST64_MIN, INT_LEAST64_MAX); verify_width (UINT_LEAST64_WIDTH, 0, UINT_LEAST64_MAX); verify_width (INT_FAST8_WIDTH, INT_FAST8_MIN, INT_FAST8_MAX); verify_width (UINT_FAST8_WIDTH, 0, UINT_FAST8_MAX); verify_width (INT_FAST16_WIDTH, INT_FAST16_MIN, INT_FAST16_MAX); verify_width (UINT_FAST16_WIDTH, 0, UINT_FAST16_MAX); verify_width (INT_FAST32_WIDTH, INT_FAST32_MIN, INT_FAST32_MAX); verify_width (UINT_FAST32_WIDTH, 0, UINT_FAST32_MAX); verify_width (INT_FAST64_WIDTH, INT_FAST64_MIN, INT_FAST64_MAX); verify_width (UINT_FAST64_WIDTH, 0, UINT_FAST64_MAX); verify_width (INTPTR_WIDTH, INTPTR_MIN, INTPTR_MAX); verify_width (UINTPTR_WIDTH, 0, UINTPTR_MAX); verify_width (INTMAX_WIDTH, INTMAX_MIN, INTMAX_MAX); verify_width (UINTMAX_WIDTH, 0, UINTMAX_MAX); verify_width (PTRDIFF_WIDTH, PTRDIFF_MIN, PTRDIFF_MAX); verify_width (SIZE_WIDTH, 0, SIZE_MAX); verify_width (WCHAR_WIDTH, WCHAR_MIN, WCHAR_MAX); #ifdef WINT_MAX verify_width (WINT_WIDTH, WINT_MIN, WINT_MAX); #endif #ifdef SIG_ATOMIC_MAX verify_width (SIG_ATOMIC_WIDTH, SIG_ATOMIC_MIN, SIG_ATOMIC_MAX); #endif int main (void) { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-stddef.c0000644000175000017500000000521313004436755017367 00000000000000/* Test of substitute. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include #include #include "verify.h" /* Check that appropriate types are defined. */ wchar_t a = 'c'; ptrdiff_t b = 1; size_t c = 2; max_align_t x; /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); /* Check that offsetof produces integer constants with correct type. */ struct d { char e; char f; }; /* Solaris 10 has a bug where offsetof is under-parenthesized, and cannot be used as an arbitrary expression. However, since it is unlikely to bite real code, we ignore that short-coming. */ /* verify (sizeof offsetof (struct d, e) == sizeof (size_t)); */ verify (sizeof (offsetof (struct d, e)) == sizeof (size_t)); verify (offsetof (struct d, e) < -1); /* Must be unsigned. */ verify (offsetof (struct d, f) == 1); /* Check max_align_t's alignment. */ verify (alignof (double) <= alignof (max_align_t)); verify (alignof (int) <= alignof (max_align_t)); verify (alignof (long double) <= alignof (max_align_t)); verify (alignof (long int) <= alignof (max_align_t)); verify (alignof (ptrdiff_t) <= alignof (max_align_t)); verify (alignof (size_t) <= alignof (max_align_t)); verify (alignof (wchar_t) <= alignof (max_align_t)); verify (alignof (struct d) <= alignof (max_align_t)); #if defined __GNUC__ || defined __IBM__ALIGNOF__ verify (__alignof__ (double) <= __alignof__ (max_align_t)); verify (__alignof__ (int) <= __alignof__ (max_align_t)); verify (__alignof__ (long double) <= __alignof__ (max_align_t)); verify (__alignof__ (long int) <= __alignof__ (max_align_t)); verify (__alignof__ (ptrdiff_t) <= __alignof__ (max_align_t)); verify (__alignof__ (size_t) <= __alignof__ (max_align_t)); verify (__alignof__ (wchar_t) <= __alignof__ (max_align_t)); verify (__alignof__ (struct d) <= __alignof__ (max_align_t)); #endif int main (void) { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-stdbool.c0000644000175000017500000000666013004436755017573 00000000000000/* Test of substitute. Copyright (C) 2002-2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ /* We want this test to succeed even when using gcc's -Werror; but to do that requires a pragma that didn't exist before 4.3.0. */ #ifndef __GNUC__ # define ADDRESS_CHECK_OKAY #elif __GNUC__ < 4 || (__GNUC__ == 4 && __GNUC_MINOR__ < 3) /* No way to silence -Waddress. */ #else # pragma GCC diagnostic ignored "-Waddress" # define ADDRESS_CHECK_OKAY #endif #include #include #ifndef bool "error: bool is not defined" #endif #ifndef false "error: false is not defined" #endif #if false "error: false is not 0" #endif #ifndef true "error: true is not defined" #endif #if true != 1 "error: true is not 1" #endif #ifndef __bool_true_false_are_defined "error: __bool_true_false_are_defined is not defined" #endif /* Several tests cannot be guaranteed with gnulib's , at least, not for all compilers and compiler options. */ #if HAVE_STDBOOL_H || 3 <= __GNUC__ struct s { _Bool s: 1; _Bool t; } s; #endif char a[true == 1 ? 1 : -1]; char b[false == 0 ? 1 : -1]; char c[__bool_true_false_are_defined == 1 ? 1 : -1]; #if HAVE_STDBOOL_H || 3 <= __GNUC__ /* See above. */ char d[(bool) 0.5 == true ? 1 : -1]; # ifdef ADDRESS_CHECK_OKAY /* Avoid gcc warning. */ /* C99 may plausibly be interpreted as not requiring support for a cast from a variable's address to bool in a static initializer. So treat it like a GCC extension. */ # ifdef __GNUC__ bool e = &s; # endif # endif char f[(_Bool) 0.0 == false ? 1 : -1]; #endif char g[true]; char h[sizeof (_Bool)]; #if HAVE_STDBOOL_H || 3 <= __GNUC__ /* See above. */ char i[sizeof s.t]; #endif enum { j = false, k = true, l = false * true, m = true * 256 }; _Bool n[m]; char o[sizeof n == m * sizeof n[0] ? 1 : -1]; char p[-1 - (_Bool) 0 < 0 && -1 - (bool) 0 < 0 ? 1 : -1]; /* Catch a bug in an HP-UX C compiler. See http://gcc.gnu.org/ml/gcc-patches/2003-12/msg02303.html http://lists.gnu.org/archive/html/bug-coreutils/2005-11/msg00161.html */ _Bool q = true; _Bool *pq = &q; int main () { int error = 0; #if HAVE_STDBOOL_H || 3 <= __GNUC__ /* See above. */ # ifdef ADDRESS_CHECK_OKAY /* Avoid gcc warning. */ /* A cast from a variable's address to bool is valid in expressions. */ { bool e1 = &s; if (!e1) error = 1; } # endif #endif /* Catch a bug in IBM AIX xlc compiler version 6.0.0.0 reported by James Lemley on 2005-10-05; see http://lists.gnu.org/archive/html/bug-coreutils/2005-10/msg00086.html This is a runtime test, since a corresponding compile-time test would rely on initializer extensions. */ { char digs[] = "0123456789"; if (&(digs + 5)[-2 + (bool) 1] != &digs[4]) error = 1; } return error; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-stdalign.c0000644000175000017500000000674413004436755017735 00000000000000/* Test of . Copyright 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paul Eggert, inspired by Bruno Haible's test-alignof.c. */ #include #include #include #include #include "verify.h" #include "macros.h" typedef long double longdouble; typedef struct { char a[1]; } struct1; typedef struct { char a[2]; } struct2; typedef struct { char a[3]; } struct3; typedef struct { char a[4]; } struct4; verify (__alignof_is_defined == 1); #ifndef alignof # error "alignof is not a macro" #endif #if __alignas_is_defined verify (__alignas_is_defined == 1); # ifndef alignas # error "alignas is not a macro" # endif /* mingw can go up only to 8. 8 is all that GNU Emacs needs, so let's limit the test to 8 for now. */ # define TEST_ALIGNMENT 8 #else # define _Alignas(alignment) # define alignas(alignment) # define TEST_ALIGNMENT 1 #endif #define CHECK_STATIC(type) \ typedef struct { char slot1; type slot2; } type##_helper; \ verify (alignof (type) == offsetof (type##_helper, slot2)); \ verify (_Alignof (type) == alignof (type)); \ const int type##_alignment = alignof (type); \ type alignas (TEST_ALIGNMENT) static_##type##_alignas; \ type _Alignas (TEST_ALIGNMENT) static_##type##_Alignas #define CHECK_ALIGNED(var) ASSERT ((uintptr_t) &(var) % TEST_ALIGNMENT == 0) CHECK_STATIC (char); CHECK_STATIC (short); CHECK_STATIC (int); CHECK_STATIC (long); #ifdef INT64_MAX CHECK_STATIC (int64_t); #endif CHECK_STATIC (float); CHECK_STATIC (double); /* CHECK_STATIC (longdouble); */ CHECK_STATIC (struct1); CHECK_STATIC (struct2); CHECK_STATIC (struct3); CHECK_STATIC (struct4); int main () { #if defined __SUNPRO_C /* Avoid a test failure due to Sun Studio Developer Bug Report #2125432. */ fputs ("Skipping test: known Sun C compiler bug\n", stderr); return 77; #else CHECK_ALIGNED (static_char_alignas); CHECK_ALIGNED (static_char_Alignas); CHECK_ALIGNED (static_short_alignas); CHECK_ALIGNED (static_short_Alignas); CHECK_ALIGNED (static_int_alignas); CHECK_ALIGNED (static_int_Alignas); CHECK_ALIGNED (static_long_alignas); CHECK_ALIGNED (static_long_Alignas); # ifdef INT64_MAX CHECK_ALIGNED (static_int64_t_alignas); CHECK_ALIGNED (static_int64_t_Alignas); # endif CHECK_ALIGNED (static_float_alignas); CHECK_ALIGNED (static_float_Alignas); CHECK_ALIGNED (static_double_alignas); CHECK_ALIGNED (static_double_Alignas); /* CHECK_ALIGNED (static_longdouble_alignas); */ /* CHECK_ALIGNED (static_longdouble_Alignas); */ CHECK_ALIGNED (static_struct1_alignas); CHECK_ALIGNED (static_struct1_Alignas); CHECK_ALIGNED (static_struct2_alignas); CHECK_ALIGNED (static_struct2_Alignas); CHECK_ALIGNED (static_struct3_alignas); CHECK_ALIGNED (static_struct3_Alignas); CHECK_ALIGNED (static_struct4_alignas); CHECK_ALIGNED (static_struct4_Alignas); return 0; #endif } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-stat.c0000644000175000017500000000313313004436755017070 00000000000000/* Tests of stat. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include /* Caution: stat may be a function-like macro. Although this signature check must pass, it may be the signature of the real (and broken) stat rather than rpl_stat. Most code should not use the address of stat. */ #include "signature.h" SIGNATURE_CHECK (stat, int, (char const *, struct stat *)); #include #include #include #include #include #include #include "same-inode.h" #include "macros.h" #define BASE "test-stat.t" #include "test-stat.h" /* Wrapper around stat, which works even if stat is a function-like macro, where test_stat_func(stat) would do the wrong thing. */ static int do_stat (char const *name, struct stat *st) { return stat (name, st); } int main (void) { return test_stat_func (do_stat, true); } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-sleep.c0000644000175000017500000000263213004436755017230 00000000000000/* Test of sleep() function. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "signature.h" SIGNATURE_CHECK (sleep, unsigned int, (unsigned int)); #include #include "macros.h" #if HAVE_DECL_ALARM static void handle_alarm (int sig) { if (sig != SIGALRM) _exit (1); } #endif int main (void) { ASSERT (sleep (1) <= 1); ASSERT (sleep (0) == 0); #if HAVE_DECL_ALARM { const unsigned int pentecost = 50 * 24 * 60 * 60; /* 50 days. */ unsigned int remaining; signal (SIGALRM, handle_alarm); alarm (1); remaining = sleep (pentecost); ASSERT (pentecost - 10 < remaining && remaining <= pentecost); } #endif return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-setlocale2.c0000644000175000017500000000334713004436755020161 00000000000000/* Test of setting the current locale. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include #include #include int main () { /* Try to set the locale by implicitly looking at the LC_ALL environment variable. */ if (setlocale (LC_ALL, "") != NULL) /* It was successful. Check whether LC_CTYPE is non-trivial. */ if (strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) { fprintf (stderr, "setlocale did not fail for implicit %s\n", getenv ("LC_ALL")); return 1; } /* Reset the locale. */ if (setlocale (LC_ALL, "C") == NULL) return 1; /* Try to set the locale by explicitly looking at the LC_ALL environment variable. */ if (setlocale (LC_ALL, getenv ("LC_ALL")) != NULL) /* It was successful. Check whether LC_CTYPE is non-trivial. */ if (strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) { fprintf (stderr, "setlocale did not fail for explicit %s\n", getenv ("LC_ALL")); return 1; } return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-setlocale1.c0000644000175000017500000000334113004436755020152 00000000000000/* Test of setting the current locale. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (setlocale, char *, (int, const char *)); #include #include #include "macros.h" int main (int argc, char *argv[]) { char *name1; char *name2; /* Try to set the locale by implicitly looking at the LC_ALL environment variable. configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; name1 = strdup (setlocale (LC_ALL, NULL)); /* Reset the locale. */ if (setlocale (LC_ALL, "C") == NULL) return 1; /* Try to set the locale by explicitly looking at the LC_ALL environment variable. configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL) return 1; name2 = strdup (setlocale (LC_ALL, NULL)); /* Test that the two results are the same. */ ASSERT (strcmp (name1, name2) == 0); free (name1); free (name2); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-setenv.c0000644000175000017500000000310613004436755017421 00000000000000/* Tests of setenv. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include #include "signature.h" SIGNATURE_CHECK (setenv, int, (char const *, char const *, int)); #include #include #include #include "macros.h" int main (void) { /* Test overwriting. */ ASSERT (setenv ("a", "==", -1) == 0); ASSERT (setenv ("a", "2", 0) == 0); ASSERT (strcmp (getenv ("a"), "==") == 0); /* Required to fail with EINVAL. */ errno = 0; ASSERT (setenv ("", "", 1) == -1); ASSERT (errno == EINVAL); errno = 0; ASSERT (setenv ("a=b", "", 0) == -1); ASSERT (errno == EINVAL); #if 0 /* glibc and gnulib's implementation guarantee this, but POSIX no longer requires it: http://austingroupbugs.net/view.php?id=185 */ errno = 0; ASSERT (setenv (NULL, "", 0) == -1); ASSERT (errno == EINVAL); #endif return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-regex.c0000644000175000017500000001702013004436755017227 00000000000000/* Test regular expressions Copyright 1996-2001, 2003-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "regex.h" #include #include #include #include #if HAVE_DECL_ALARM # include # include #endif #include "localcharset.h" int main (void) { int result = 0; static struct re_pattern_buffer regex; unsigned char folded_chars[UCHAR_MAX + 1]; int i; const char *s; struct re_registers regs; #if HAVE_DECL_ALARM /* Some builds of glibc go into an infinite loop on this test. */ int alarm_value = 2; signal (SIGALRM, SIG_DFL); alarm (alarm_value); #endif if (setlocale (LC_ALL, "en_US.UTF-8")) { { /* http://sourceware.org/ml/libc-hacker/2006-09/msg00008.html This test needs valgrind to catch the bug on Debian GNU/Linux 3.1 x86, but it might catch the bug better on other platforms and it shouldn't hurt to try the test here. */ static char const pat[] = "insert into"; static char const data[] = "\xFF\0\x12\xA2\xAA\xC4\xB1,K\x12\xC4\xB1*\xACK"; re_set_syntax (RE_SYNTAX_GREP | RE_HAT_LISTS_NOT_NEWLINE | RE_ICASE); memset (®ex, 0, sizeof regex); s = re_compile_pattern (pat, sizeof pat - 1, ®ex); if (s) result |= 1; else { memset (®s, 0, sizeof regs); if (re_search (®ex, data, sizeof data - 1, 0, sizeof data - 1, ®s) != -1) result |= 1; regfree (®ex); free (regs.start); free (regs.end); } } /* Check whether it's really a UTF-8 locale. On mingw, the setlocale call succeeds but returns "English_United States.1252", with locale_charset() returning "CP1252". */ if (strcmp (locale_charset (), "UTF-8") == 0) { /* This test is from glibc bug 15078. The test case is from Andreas Schwab in . */ static char const pat[] = "[^x]x"; static char const data[] = /* */ "\xe1\x80\x80" "\xe1\x80\xbb" "\xe1\x80\xbd" "\xe1\x80\x94" "\xe1\x80\xba" "\xe1\x80\xaf" "\xe1\x80\x95" "\xe1\x80\xba" "x"; re_set_syntax (0); memset (®ex, 0, sizeof regex); s = re_compile_pattern (pat, sizeof pat - 1, ®ex); if (s) result |= 1; else { memset (®s, 0, sizeof regs); i = re_search (®ex, data, sizeof data - 1, 0, sizeof data - 1, 0); if (i != 0 && i != 21) result |= 1; regfree (®ex); free (regs.start); free (regs.end); } } if (! setlocale (LC_ALL, "C")) return 1; } /* This test is from glibc bug 3957, reported by Andrew Mackey. */ re_set_syntax (RE_SYNTAX_EGREP | RE_HAT_LISTS_NOT_NEWLINE); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("a[^x]b", 6, ®ex); if (s) result |= 2; /* This should fail, but succeeds for glibc-2.5. */ else { memset (®s, 0, sizeof regs); if (re_search (®ex, "a\nb", 3, 0, 3, ®s) != -1) result |= 2; regfree (®ex); free (regs.start); free (regs.end); } /* This regular expression is from Spencer ere test number 75 in grep-2.3. */ re_set_syntax (RE_SYNTAX_POSIX_EGREP); memset (®ex, 0, sizeof regex); for (i = 0; i <= UCHAR_MAX; i++) folded_chars[i] = i; regex.translate = folded_chars; s = re_compile_pattern ("a[[:@:>@:]]b\n", 11, ®ex); /* This should fail with _Invalid character class name_ error. */ if (!s) { result |= 4; regfree (®ex); } /* Ensure that [b-a] is diagnosed as invalid, when using RE_NO_EMPTY_RANGES. */ re_set_syntax (RE_SYNTAX_POSIX_EGREP | RE_NO_EMPTY_RANGES); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("a[b-a]", 6, ®ex); if (s == 0) { result |= 8; regfree (®ex); } /* This should succeed, but does not for glibc-2.1.3. */ memset (®ex, 0, sizeof regex); s = re_compile_pattern ("{1", 2, ®ex); if (s) result |= 8; else regfree (®ex); /* The following example is derived from a problem report against gawk from Jorge Stolfi . */ memset (®ex, 0, sizeof regex); s = re_compile_pattern ("[an\371]*n", 7, ®ex); if (s) result |= 8; /* This should match, but does not for glibc-2.2.1. */ else { memset (®s, 0, sizeof regs); if (re_match (®ex, "an", 2, 0, ®s) != 2) result |= 8; regfree (®ex); free (regs.start); free (regs.end); } memset (®ex, 0, sizeof regex); s = re_compile_pattern ("x", 1, ®ex); if (s) result |= 8; /* glibc-2.2.93 does not work with a negative RANGE argument. */ else { memset (®s, 0, sizeof regs); if (re_search (®ex, "wxy", 3, 2, -2, ®s) != 1) result |= 8; regfree (®ex); free (regs.start); free (regs.end); } /* The version of regex.c in older versions of gnulib ignored RE_ICASE. Detect that problem too. */ re_set_syntax (RE_SYNTAX_EMACS | RE_ICASE); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("x", 1, ®ex); if (s) result |= 16; else { memset (®s, 0, sizeof regs); if (re_search (®ex, "WXY", 3, 0, 3, ®s) < 0) result |= 16; regfree (®ex); free (regs.start); free (regs.end); } /* Catch a bug reported by Vin Shelton in http://lists.gnu.org/archive/html/bug-coreutils/2007-06/msg00089.html */ re_set_syntax (RE_SYNTAX_POSIX_BASIC & ~RE_CONTEXT_INVALID_DUP & ~RE_NO_EMPTY_RANGES); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("[[:alnum:]_-]\\\\+$", 16, ®ex); if (s) result |= 32; else regfree (®ex); /* REG_STARTEND was added to glibc on 2004-01-15. Reject older versions. */ if (! REG_STARTEND) result |= 64; #if 0 /* It would be nice to reject hosts whose regoff_t values are too narrow (including glibc on hosts with 64-bit ptrdiff_t and 32-bit int), but we should wait until glibc implements this feature. Otherwise, support for equivalence classes and multibyte collation symbols would always be broken except when compiling --without-included-regex. */ if (sizeof (regoff_t) < sizeof (ptrdiff_t) || sizeof (regoff_t) < sizeof (ssize_t)) result |= 64; #endif return result; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-rawmemchr.c0000644000175000017500000000475413004436755020114 00000000000000/* * Copyright (C) 2008-2016 Free Software Foundation, Inc. * Written by Eric Blake and Bruno Haible * * This program is free software: you can redistribute it and/or modify * it under the terms of the GNU General Public License as published by * the Free Software Foundation; either version 3 of the License, or * (at your option) any later version. * * This program is distributed in the hope that it will be useful, * but WITHOUT ANY WARRANTY; without even the implied warranty of * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * GNU General Public License for more details. * * You should have received a copy of the GNU General Public License * along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (rawmemchr, void *, (void const *, int)); #include #include "zerosize-ptr.h" #include "macros.h" /* Calculating void * + int is not portable, so this wrapper converts to char * to make the tests easier to write. */ #define RAWMEMCHR (char *) rawmemchr int main (void) { size_t n = 0x100000; char *input = malloc (n + 1); ASSERT (input); input[0] = 'a'; input[1] = 'b'; memset (input + 2, 'c', 1024); memset (input + 1026, 'd', n - 1028); input[n - 2] = 'e'; input[n - 1] = 'a'; input[n] = '\0'; /* Basic behavior tests. */ ASSERT (RAWMEMCHR (input, 'a') == input); ASSERT (RAWMEMCHR (input, 'b') == input + 1); ASSERT (RAWMEMCHR (input, 'c') == input + 2); ASSERT (RAWMEMCHR (input, 'd') == input + 1026); ASSERT (RAWMEMCHR (input + 1, 'a') == input + n - 1); ASSERT (RAWMEMCHR (input + 1, 'e') == input + n - 2); ASSERT (RAWMEMCHR (input + 1, 0x789abc00 | 'e') == input + n - 2); ASSERT (RAWMEMCHR (input, '\0') == input + n); /* Alignment tests. */ { int i, j; for (i = 0; i < 32; i++) { for (j = 0; j < 256; j++) input[i + j] = j; for (j = 0; j < 256; j++) { ASSERT (RAWMEMCHR (input + i, j) == input + i + j); } } } /* Ensure that no unaligned oversized reads occur. */ { char *page_boundary = (char *) zerosize_ptr (); size_t i; if (!page_boundary) page_boundary = input + 4096; memset (page_boundary - 512, '1', 511); page_boundary[-1] = '2'; for (i = 1; i <= 512; i++) ASSERT (RAWMEMCHR (page_boundary - i, (i * 0x01010100) | '2') == page_boundary - 1); } free (input); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-pathmax.c0000644000175000017500000000170313004436755017560 00000000000000/* Test of "pathmax.h". Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2011. */ #include #include "pathmax.h" /* Check that PATH_MAX is a constant if it is defined. */ #ifdef PATH_MAX int a = PATH_MAX; #endif int main (void) { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-open.c0000644000175000017500000000214713004436755017062 00000000000000/* Test of opening a file descriptor. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "signature.h" SIGNATURE_CHECK (open, int, (char const *, int, ...)); #include #include #include #include #include "macros.h" #define BASE "test-open.t" #include "test-open.h" int main (void) { return test_open (open, true); } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-nl_langinfo.c0000644000175000017500000001110013004436755020374 00000000000000/* Test of nl_langinfo replacement. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ #include #include #include "signature.h" SIGNATURE_CHECK (nl_langinfo, char *, (nl_item)); #include #include #include #include "c-strcase.h" #include "macros.h" /* For GCC >= 4.3, silence the warnings "comparison of unsigned expression >= 0 is always true" in this file. */ #if __GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 3) # pragma GCC diagnostic ignored "-Wtype-limits" #endif int main (int argc, char *argv[]) { int pass = atoi (argv[1]); /* pass locale 0 C 1 traditional French locale 2 French UTF-8 locale */ setlocale (LC_ALL, ""); /* nl_langinfo items of the LC_CTYPE category */ ASSERT (strlen (nl_langinfo (CODESET)) > 0); if (pass == 2) { const char *codeset = nl_langinfo (CODESET); ASSERT (c_strcasecmp (codeset, "UTF-8") == 0 || c_strcasecmp (codeset, "UTF8") == 0); } /* nl_langinfo items of the LC_NUMERIC category */ ASSERT (strlen (nl_langinfo (RADIXCHAR)) > 0); ASSERT (strlen (nl_langinfo (THOUSEP)) >= 0); /* nl_langinfo items of the LC_TIME category */ ASSERT (strlen (nl_langinfo (D_T_FMT)) > 0); ASSERT (strlen (nl_langinfo (D_FMT)) > 0); ASSERT (strlen (nl_langinfo (T_FMT)) > 0); ASSERT (strlen (nl_langinfo (T_FMT_AMPM)) >= (pass == 0 ? 1 : 0)); ASSERT (strlen (nl_langinfo (AM_STR)) >= (pass == 0 ? 1 : 0)); ASSERT (strlen (nl_langinfo (PM_STR)) >= (pass == 0 ? 1 : 0)); ASSERT (strlen (nl_langinfo (DAY_1)) > 0); ASSERT (strlen (nl_langinfo (DAY_2)) > 0); ASSERT (strlen (nl_langinfo (DAY_3)) > 0); ASSERT (strlen (nl_langinfo (DAY_4)) > 0); ASSERT (strlen (nl_langinfo (DAY_5)) > 0); ASSERT (strlen (nl_langinfo (DAY_6)) > 0); ASSERT (strlen (nl_langinfo (DAY_7)) > 0); ASSERT (strlen (nl_langinfo (ABDAY_1)) > 0); ASSERT (strlen (nl_langinfo (ABDAY_2)) > 0); ASSERT (strlen (nl_langinfo (ABDAY_3)) > 0); ASSERT (strlen (nl_langinfo (ABDAY_4)) > 0); ASSERT (strlen (nl_langinfo (ABDAY_5)) > 0); ASSERT (strlen (nl_langinfo (ABDAY_6)) > 0); ASSERT (strlen (nl_langinfo (ABDAY_7)) > 0); ASSERT (strlen (nl_langinfo (MON_1)) > 0); ASSERT (strlen (nl_langinfo (MON_2)) > 0); ASSERT (strlen (nl_langinfo (MON_3)) > 0); ASSERT (strlen (nl_langinfo (MON_4)) > 0); ASSERT (strlen (nl_langinfo (MON_5)) > 0); ASSERT (strlen (nl_langinfo (MON_6)) > 0); ASSERT (strlen (nl_langinfo (MON_7)) > 0); ASSERT (strlen (nl_langinfo (MON_8)) > 0); ASSERT (strlen (nl_langinfo (MON_9)) > 0); ASSERT (strlen (nl_langinfo (MON_10)) > 0); ASSERT (strlen (nl_langinfo (MON_11)) > 0); ASSERT (strlen (nl_langinfo (MON_12)) > 0); ASSERT (strlen (nl_langinfo (ABMON_1)) > 0); ASSERT (strlen (nl_langinfo (ABMON_2)) > 0); ASSERT (strlen (nl_langinfo (ABMON_3)) > 0); ASSERT (strlen (nl_langinfo (ABMON_4)) > 0); ASSERT (strlen (nl_langinfo (ABMON_5)) > 0); ASSERT (strlen (nl_langinfo (ABMON_6)) > 0); ASSERT (strlen (nl_langinfo (ABMON_7)) > 0); ASSERT (strlen (nl_langinfo (ABMON_8)) > 0); ASSERT (strlen (nl_langinfo (ABMON_9)) > 0); ASSERT (strlen (nl_langinfo (ABMON_10)) > 0); ASSERT (strlen (nl_langinfo (ABMON_11)) > 0); ASSERT (strlen (nl_langinfo (ABMON_12)) > 0); ASSERT (strlen (nl_langinfo (ERA)) >= 0); ASSERT (strlen (nl_langinfo (ERA_D_FMT)) >= 0); ASSERT (strlen (nl_langinfo (ERA_D_T_FMT)) >= 0); ASSERT (strlen (nl_langinfo (ERA_T_FMT)) >= 0); ASSERT (nl_langinfo (ALT_DIGITS) != NULL); /* nl_langinfo items of the LC_MONETARY category */ { const char *currency = nl_langinfo (CRNCYSTR); ASSERT (strlen (currency) >= 0); #if !defined __NetBSD__ if (pass > 0) ASSERT (strlen (currency) >= 1); #endif } /* nl_langinfo items of the LC_MESSAGES category */ ASSERT (strlen (nl_langinfo (YESEXPR)) > 0); ASSERT (strlen (nl_langinfo (NOEXPR)) > 0); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-memchr.c0000644000175000017500000000731213004436755017373 00000000000000/* * Copyright (C) 2008-2016 Free Software Foundation, Inc. * Written by Eric Blake and Bruno Haible * * This program is free software: you can redistribute it and/or modify * it under the terms of the GNU General Public License as published by * the Free Software Foundation; either version 3 of the License, or * (at your option) any later version. * * This program is distributed in the hope that it will be useful, * but WITHOUT ANY WARRANTY; without even the implied warranty of * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * GNU General Public License for more details. * * You should have received a copy of the GNU General Public License * along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (memchr, void *, (void const *, int, size_t)); #include #include "zerosize-ptr.h" #include "macros.h" /* Calculating void * + int is not portable, so this wrapper converts to char * to make the tests easier to write. */ #define MEMCHR (char *) memchr int main (void) { size_t n = 0x100000; char *input = malloc (n); ASSERT (input); input[0] = 'a'; input[1] = 'b'; memset (input + 2, 'c', 1024); memset (input + 1026, 'd', n - 1028); input[n - 2] = 'e'; input[n - 1] = 'a'; /* Basic behavior tests. */ ASSERT (MEMCHR (input, 'a', n) == input); ASSERT (MEMCHR (input, 'a', 0) == NULL); ASSERT (MEMCHR (zerosize_ptr (), 'a', 0) == NULL); ASSERT (MEMCHR (input, 'b', n) == input + 1); ASSERT (MEMCHR (input, 'c', n) == input + 2); ASSERT (MEMCHR (input, 'd', n) == input + 1026); ASSERT (MEMCHR (input + 1, 'a', n - 1) == input + n - 1); ASSERT (MEMCHR (input + 1, 'e', n - 1) == input + n - 2); ASSERT (MEMCHR (input + 1, 0x789abc00 | 'e', n - 1) == input + n - 2); ASSERT (MEMCHR (input, 'f', n) == NULL); ASSERT (MEMCHR (input, '\0', n) == NULL); /* Check that a very long haystack is handled quickly if the byte is found near the beginning. */ { size_t repeat = 10000; for (; repeat > 0; repeat--) { ASSERT (MEMCHR (input, 'c', n) == input + 2); } } /* Alignment tests. */ { int i, j; for (i = 0; i < 32; i++) { for (j = 0; j < 256; j++) input[i + j] = j; for (j = 0; j < 256; j++) { ASSERT (MEMCHR (input + i, j, 256) == input + i + j); } } } /* Check that memchr() does not read past the first occurrence of the byte being searched. See the Austin Group's clarification . Test both '\0' and something else, since some implementations special-case searching for NUL. */ { char *page_boundary = (char *) zerosize_ptr (); /* Too small, and we miss cache line boundary tests; too large, and the test takes cubically longer to complete. */ int limit = 257; if (page_boundary != NULL) { for (n = 1; n <= limit; n++) { char *mem = page_boundary - n; memset (mem, 'X', n); ASSERT (MEMCHR (mem, 'U', n) == NULL); ASSERT (MEMCHR (mem, 0, n) == NULL); { size_t i; size_t k; for (i = 0; i < n; i++) { mem[i] = 'U'; for (k = i + 1; k < n + limit; k++) ASSERT (MEMCHR (mem, 'U', k) == mem + i); mem[i] = 0; for (k = i + 1; k < n + limit; k++) ASSERT (MEMCHR (mem, 0, k) == mem + i); mem[i] = 'X'; } } } } } free (input); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-mbsinit.c0000644000175000017500000000267613004436755017575 00000000000000/* Test of test for initial conversion state. Copyright (C) 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include #include "signature.h" SIGNATURE_CHECK (mbsinit, int, (const mbstate_t *)); #include #include "macros.h" int main (int argc, char *argv[]) { static mbstate_t state; ASSERT (mbsinit (NULL)); ASSERT (mbsinit (&state)); if (argc > 1) { static const char input[1] = "\303"; wchar_t wc; size_t ret; /* configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (!mbsinit (&state)); } return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-mbrtowc-w32.c0000644000175000017500000005411513004436755020211 00000000000000/* Test of conversion of multibyte character to wide character. Copyright (C) 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include #include #include #include #include #include "macros.h" #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ static int test_one_locale (const char *name, int codepage) { mbstate_t state; wchar_t wc; size_t ret; # if 1 /* Portable code to set the locale. */ { char name_with_codepage[1024]; sprintf (name_with_codepage, "%s.%d", name, codepage); /* Set the locale. */ if (setlocale (LC_ALL, name_with_codepage) == NULL) return 77; } # else /* Hacky way to set a locale.codepage combination that setlocale() refuses to set. */ { /* Codepage of the current locale, set with setlocale(). Not necessarily the same as GetACP(). */ extern __declspec(dllimport) unsigned int __lc_codepage; /* Set the locale. */ if (setlocale (LC_ALL, name) == NULL) return 77; /* Clobber the codepage and MB_CUR_MAX, both set by setlocale(). */ __lc_codepage = codepage; switch (codepage) { case 1252: case 1256: MB_CUR_MAX = 1; break; case 932: case 950: case 936: MB_CUR_MAX = 2; break; case 54936: case 65001: MB_CUR_MAX = 4; break; } /* Test whether the codepage is really available. */ memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, " ", 1, &state) == (size_t)(-1)) return 77; } # endif /* Test zero-length input. */ { memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "x", 0, &state); /* gnulib's implementation returns (size_t)(-2). The AIX 5.1 implementation returns (size_t)(-1). glibc's implementation returns 0. */ ASSERT (ret == (size_t)(-2) || ret == (size_t)(-1) || ret == 0); ASSERT (mbsinit (&state)); } /* Test NUL byte input. */ { memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "", 1, &state); ASSERT (ret == 0); ASSERT (wc == 0); ASSERT (mbsinit (&state)); ret = mbrtowc (NULL, "", 1, &state); ASSERT (ret == 0); ASSERT (mbsinit (&state)); } /* Test single-byte input. */ { int c; char buf[1]; memset (&state, '\0', sizeof (mbstate_t)); for (c = 0; c < 0x100; c++) switch (c) { case '\t': case '\v': case '\f': case ' ': case '!': case '"': case '#': case '%': case '&': case '\'': case '(': case ')': case '*': case '+': case ',': case '-': case '.': case '/': case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': case ':': case ';': case '<': case '=': case '>': case '?': case 'A': case 'B': case 'C': case 'D': case 'E': case 'F': case 'G': case 'H': case 'I': case 'J': case 'K': case 'L': case 'M': case 'N': case 'O': case 'P': case 'Q': case 'R': case 'S': case 'T': case 'U': case 'V': case 'W': case 'X': case 'Y': case 'Z': case '[': case '\\': case ']': case '^': case '_': case 'a': case 'b': case 'c': case 'd': case 'e': case 'f': case 'g': case 'h': case 'i': case 'j': case 'k': case 'l': case 'm': case 'n': case 'o': case 'p': case 'q': case 'r': case 's': case 't': case 'u': case 'v': case 'w': case 'x': case 'y': case 'z': case '{': case '|': case '}': case '~': /* c is in the ISO C "basic character set". */ buf[0] = c; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, buf, 1, &state); ASSERT (ret == 1); ASSERT (wc == c); ASSERT (mbsinit (&state)); ret = mbrtowc (NULL, buf, 1, &state); ASSERT (ret == 1); ASSERT (mbsinit (&state)); break; } } /* Test special calling convention, passing a NULL pointer. */ { memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, NULL, 5, &state); ASSERT (ret == 0); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (mbsinit (&state)); } switch (codepage) { case 1252: /* Locale encoding is CP1252, an extension of ISO-8859-1. */ { char input[] = "B\374\337er"; /* "Büßer" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'B'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 1, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == (unsigned char) '\374'); ASSERT (wc == 0x00FC); ASSERT (mbsinit (&state)); input[1] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 2, 3, &state); ASSERT (ret == 1); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 2, 3, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == (unsigned char) '\337'); ASSERT (wc == 0x00DF); ASSERT (mbsinit (&state)); input[2] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 2, &state); ASSERT (ret == 1); ASSERT (wc == 'e'); ASSERT (mbsinit (&state)); input[3] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 4, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'r'); ASSERT (mbsinit (&state)); } return 0; case 1256: /* Locale encoding is CP1256, not the same as ISO-8859-6. */ { char input[] = "x\302\341\346y"; /* "xآلوy" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'x'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 1, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == (unsigned char) '\302'); ASSERT (wc == 0x0622); ASSERT (mbsinit (&state)); input[1] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 2, 3, &state); ASSERT (ret == 1); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 2, 3, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == (unsigned char) '\341'); ASSERT (wc == 0x0644); ASSERT (mbsinit (&state)); input[2] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 2, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == (unsigned char) '\346'); ASSERT (wc == 0x0648); ASSERT (mbsinit (&state)); input[3] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 4, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'y'); ASSERT (mbsinit (&state)); } return 0; case 932: /* Locale encoding is CP932, similar to Shift_JIS. */ { char input[] = "<\223\372\226\173\214\352>"; /* "<日本語>" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == '<'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 2, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x65E5); ASSERT (mbsinit (&state)); input[1] = '\0'; input[2] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[3] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 4, 4, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x672C); ASSERT (mbsinit (&state)); input[4] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x8A9E); ASSERT (mbsinit (&state)); input[5] = '\0'; input[6] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 7, 1, &state); ASSERT (ret == 1); ASSERT (wc == '>'); ASSERT (mbsinit (&state)); /* Test some invalid input. */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\377", 1, &state); /* 0xFF */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\225\377", 2, &state); /* 0x95 0xFF */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); } return 0; case 950: /* Locale encoding is CP950, similar to Big5. */ { char input[] = "<\244\351\245\273\273\171>"; /* "<日本語>" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == '<'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 2, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x65E5); ASSERT (mbsinit (&state)); input[1] = '\0'; input[2] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[3] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 4, 4, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x672C); ASSERT (mbsinit (&state)); input[4] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x8A9E); ASSERT (mbsinit (&state)); input[5] = '\0'; input[6] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 7, 1, &state); ASSERT (ret == 1); ASSERT (wc == '>'); ASSERT (mbsinit (&state)); /* Test some invalid input. */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\377", 1, &state); /* 0xFF */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\225\377", 2, &state); /* 0x95 0xFF */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); } return 0; case 936: /* Locale encoding is CP936 = GBK, an extension of GB2312. */ { char input[] = "<\310\325\261\276\325\132>"; /* "<日本語>" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == '<'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 2, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x65E5); ASSERT (mbsinit (&state)); input[1] = '\0'; input[2] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[3] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 4, 4, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x672C); ASSERT (mbsinit (&state)); input[4] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x8A9E); ASSERT (mbsinit (&state)); input[5] = '\0'; input[6] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 7, 1, &state); ASSERT (ret == 1); ASSERT (wc == '>'); ASSERT (mbsinit (&state)); /* Test some invalid input. */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\377", 1, &state); /* 0xFF */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\225\377", 2, &state); /* 0x95 0xFF */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); } return 0; case 54936: /* Locale encoding is CP54936 = GB18030. */ { char input[] = "B\250\271\201\060\211\070er"; /* "Büßer" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'B'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[1] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 2, 7, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x00FC); ASSERT (mbsinit (&state)); input[2] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 3, 6, &state); ASSERT (ret == 4); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 6, &state); ASSERT (ret == 4); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x00DF); ASSERT (mbsinit (&state)); input[3] = '\0'; input[4] = '\0'; input[5] = '\0'; input[6] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 7, 2, &state); ASSERT (ret == 1); ASSERT (wc == 'e'); ASSERT (mbsinit (&state)); input[5] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 8, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'r'); ASSERT (mbsinit (&state)); /* Test some invalid input. */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\377", 1, &state); /* 0xFF */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\225\377", 2, &state); /* 0x95 0xFF */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\201\045", 2, &state); /* 0x81 0x25 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\201\060\377", 3, &state); /* 0x81 0x30 0xFF */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\201\060\377\064", 4, &state); /* 0x81 0x30 0xFF 0x34 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\201\060\211\072", 4, &state); /* 0x81 0x30 0x89 0x3A */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); } return 0; case 65001: /* Locale encoding is CP65001 = UTF-8. */ { char input[] = "B\303\274\303\237er"; /* "Büßer" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'B'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[1] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 2, 5, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x00FC); ASSERT (mbsinit (&state)); input[2] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 3, 4, &state); ASSERT (ret == 2); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 4, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x00DF); ASSERT (mbsinit (&state)); input[3] = '\0'; input[4] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 5, 2, &state); ASSERT (ret == 1); ASSERT (wc == 'e'); ASSERT (mbsinit (&state)); input[5] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 6, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'r'); ASSERT (mbsinit (&state)); /* Test some invalid input. */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\377", 1, &state); /* 0xFF */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\303\300", 2, &state); /* 0xC3 0xC0 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\343\300", 2, &state); /* 0xE3 0xC0 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\343\300\200", 3, &state); /* 0xE3 0xC0 0x80 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\343\200\300", 3, &state); /* 0xE3 0x80 0xC0 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\363\300", 2, &state); /* 0xF3 0xC0 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\363\300\200\200", 4, &state); /* 0xF3 0xC0 0x80 0x80 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\363\200\300", 3, &state); /* 0xF3 0x80 0xC0 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\363\200\300\200", 4, &state); /* 0xF3 0x80 0xC0 0x80 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\363\200\200\300", 4, &state); /* 0xF3 0x80 0x80 0xC0 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); } return 0; default: return 1; } } int main (int argc, char *argv[]) { int codepage = atoi (argv[argc - 1]); int result; int i; result = 77; for (i = 1; i < argc - 1; i++) { int ret = test_one_locale (argv[i], codepage); if (ret != 77) result = ret; } if (result == 77) { fprintf (stderr, "Skipping test: found no locale with codepage %d\n", codepage); } return result; } #else int main (int argc, char *argv[]) { fputs ("Skipping test: not a native Windows system\n", stderr); return 77; } #endif gnuastro-0.2.33-8a3b/bootstrapped/tests/test-mbrtowc.c0000644000175000017500000002522613004436755017601 00000000000000/* Test of conversion of multibyte character to wide character. Copyright (C) 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include #include "signature.h" SIGNATURE_CHECK (mbrtowc, size_t, (wchar_t *, char const *, size_t, mbstate_t *)); #include #include #include #include "macros.h" int main (int argc, char *argv[]) { mbstate_t state; wchar_t wc; size_t ret; /* configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; /* Test zero-length input. */ { memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "x", 0, &state); ASSERT (ret == (size_t)(-2)); ASSERT (mbsinit (&state)); } /* Test NUL byte input. */ { memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "", 1, &state); ASSERT (ret == 0); ASSERT (wc == 0); ASSERT (mbsinit (&state)); ret = mbrtowc (NULL, "", 1, &state); ASSERT (ret == 0); ASSERT (mbsinit (&state)); } /* Test single-byte input. */ { int c; char buf[1]; memset (&state, '\0', sizeof (mbstate_t)); for (c = 0; c < 0x100; c++) switch (c) { default: if (! (c && 1 < argc && argv[1][0] == '5')) break; /* Fall through. */ case '\t': case '\v': case '\f': case ' ': case '!': case '"': case '#': case '%': case '&': case '\'': case '(': case ')': case '*': case '+': case ',': case '-': case '.': case '/': case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': case ':': case ';': case '<': case '=': case '>': case '?': case 'A': case 'B': case 'C': case 'D': case 'E': case 'F': case 'G': case 'H': case 'I': case 'J': case 'K': case 'L': case 'M': case 'N': case 'O': case 'P': case 'Q': case 'R': case 'S': case 'T': case 'U': case 'V': case 'W': case 'X': case 'Y': case 'Z': case '[': case '\\': case ']': case '^': case '_': case 'a': case 'b': case 'c': case 'd': case 'e': case 'f': case 'g': case 'h': case 'i': case 'j': case 'k': case 'l': case 'm': case 'n': case 'o': case 'p': case 'q': case 'r': case 's': case 't': case 'u': case 'v': case 'w': case 'x': case 'y': case 'z': case '{': case '|': case '}': case '~': /* c is in the ISO C "basic character set", or argv[1] starts with '5' so we are testing all nonnull bytes. */ buf[0] = c; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, buf, 1, &state); ASSERT (ret == 1); ASSERT (wc == c); ASSERT (mbsinit (&state)); ret = mbrtowc (NULL, buf, 1, &state); ASSERT (ret == 1); ASSERT (mbsinit (&state)); break; } } /* Test special calling convention, passing a NULL pointer. */ { memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, NULL, 5, &state); ASSERT (ret == 0); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (mbsinit (&state)); } if (argc > 1) switch (argv[1][0]) { case '1': /* Locale encoding is ISO-8859-1 or ISO-8859-15. */ { char input[] = "B\374\337er"; /* "Büßer" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'B'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 1, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == (unsigned char) '\374'); ASSERT (mbsinit (&state)); input[1] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 2, 3, &state); ASSERT (ret == 1); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 2, 3, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == (unsigned char) '\337'); ASSERT (mbsinit (&state)); input[2] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 2, &state); ASSERT (ret == 1); ASSERT (wc == 'e'); ASSERT (mbsinit (&state)); input[3] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 4, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'r'); ASSERT (mbsinit (&state)); } return 0; case '2': /* Locale encoding is UTF-8. */ { char input[] = "B\303\274\303\237er"; /* "Büßer" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'B'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[1] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 2, 5, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (mbsinit (&state)); input[2] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 3, 4, &state); ASSERT (ret == 2); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 4, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (mbsinit (&state)); input[3] = '\0'; input[4] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 5, 2, &state); ASSERT (ret == 1); ASSERT (wc == 'e'); ASSERT (mbsinit (&state)); input[5] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 6, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'r'); ASSERT (mbsinit (&state)); } return 0; case '3': /* Locale encoding is EUC-JP. */ { char input[] = "<\306\374\313\334\270\354>"; /* "<日本語>" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == '<'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 2, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (mbsinit (&state)); input[1] = '\0'; input[2] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[3] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 4, 4, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (mbsinit (&state)); input[4] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (mbsinit (&state)); input[5] = '\0'; input[6] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 7, 1, &state); ASSERT (ret == 1); ASSERT (wc == '>'); ASSERT (mbsinit (&state)); } return 0; case '4': /* Locale encoding is GB18030. */ { char input[] = "B\250\271\201\060\211\070er"; /* "Büßer" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'B'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[1] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 2, 7, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (mbsinit (&state)); input[2] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 3, 6, &state); ASSERT (ret == 4); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 6, &state); ASSERT (ret == 4); ASSERT (wctob (wc) == EOF); ASSERT (mbsinit (&state)); input[3] = '\0'; input[4] = '\0'; input[5] = '\0'; input[6] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 7, 2, &state); ASSERT (ret == 1); ASSERT (wc == 'e'); ASSERT (mbsinit (&state)); input[5] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 8, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'r'); ASSERT (mbsinit (&state)); } return 0; case '5': /* C locale; tested above. */ return 0; } return 1; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-math.c0000644000175000017500000000435013004436755017050 00000000000000/* Test of substitute. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #ifndef NAN # error NAN should be defined choke me #endif #ifndef HUGE_VALF # error HUGE_VALF should be defined choke me #endif #ifndef HUGE_VAL # error HUGE_VAL should be defined choke me #endif #ifndef HUGE_VALL # error HUGE_VALL should be defined choke me #endif #ifndef FP_ILOGB0 # error FP_ILOGB0 should be defined choke me #endif #ifndef FP_ILOGBNAN # error FP_ILOGBNAN should be defined choke me #endif #include #include "macros.h" #if 0 /* Check that NAN expands into a constant expression. */ static float n = NAN; #endif /* Compare two numbers with ==. This is a separate function because IRIX 6.5 "cc -O" miscompiles an 'x == x' test. */ static int numeric_equalf (float x, float y) { return x == y; } static int numeric_equald (double x, double y) { return x == y; } static int numeric_equall (long double x, long double y) { return x == y; } int main (void) { double d = NAN; double zero = 0.0; ASSERT (!numeric_equald (d, d)); d = HUGE_VAL; ASSERT (numeric_equald (d, 1.0 / zero)); ASSERT (numeric_equalf (HUGE_VALF, HUGE_VALF + HUGE_VALF)); ASSERT (numeric_equald (HUGE_VAL, HUGE_VAL + HUGE_VAL)); ASSERT (numeric_equall (HUGE_VALL, HUGE_VALL + HUGE_VALL)); /* Check the value of FP_ILOGB0. */ ASSERT (FP_ILOGB0 == INT_MIN || FP_ILOGB0 == - INT_MAX); /* Check the value of FP_ILOGBNAN. */ ASSERT (FP_ILOGBNAN == INT_MIN || FP_ILOGBNAN == INT_MAX); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-malloca.c0000644000175000017500000000306013004436755017524 00000000000000/* Test of safe automatic memory allocation. Copyright (C) 2005, 2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2005. */ #include #include "malloca.h" #include static void do_allocation (int n) { void *ptr = malloca (n); freea (ptr); safe_alloca (n); } void (*func) (int) = do_allocation; int main () { int i; /* This slows down malloc a lot. */ unsetenv ("MALLOC_PERTURB_"); /* Repeat a lot of times, to make sure there's no memory leak. */ for (i = 0; i < 50000; i++) { /* Try various values. n = 0 gave a crash on Alpha with gcc-2.5.8. Some versions of Mac OS X have a stack size limit of 512 KB. */ func (34); func (134); func (399); func (510823); func (129321); func (0); func (4070); func (4095); func (1); func (16582); } return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-malloc-gnu.c0000644000175000017500000000160313004436755020153 00000000000000/* Test of malloc function. Copyright (C) 2010-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include int main () { /* Check that malloc (0) is not a NULL pointer. */ if (malloc (0) == NULL) return 1; return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-lstat.c0000644000175000017500000000340513004436755017246 00000000000000/* Test of lstat() function. Copyright (C) 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Simon Josefsson, 2008; and Eric Blake, 2009. */ #include #include /* Caution: lstat may be a function-like macro. Although this signature check must pass, it may be the signature of the real (and broken) lstat rather than rpl_lstat. Most code should not use the address of lstat. */ #include "signature.h" SIGNATURE_CHECK (lstat, int, (char const *, struct stat *)); #include #include #include #include #include #include #include "same-inode.h" #include "ignore-value.h" #include "macros.h" #define BASE "test-lstat.t" #include "test-lstat.h" /* Wrapper around lstat, which works even if lstat is a function-like macro, where test_lstat_func(lstat) would do the wrong thing. */ static int do_lstat (char const *name, struct stat *st) { return lstat (name, st); } int main (void) { /* Remove any leftovers from a previous partial run. */ ignore_value (system ("rm -rf " BASE "*")); return test_lstat_func (do_lstat, true); } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-lock.c0000644000175000017500000003630013004436755017047 00000000000000/* Test of locking in multithreaded situations. Copyright (C) 2005, 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2005. */ #include #if USE_POSIX_THREADS || USE_SOLARIS_THREADS || USE_PTH_THREADS || USE_WINDOWS_THREADS #if USE_POSIX_THREADS # define TEST_POSIX_THREADS 1 #endif #if USE_SOLARIS_THREADS # define TEST_SOLARIS_THREADS 1 #endif #if USE_PTH_THREADS # define TEST_PTH_THREADS 1 #endif #if USE_WINDOWS_THREADS # define TEST_WINDOWS_THREADS 1 #endif /* Whether to enable locking. Uncomment this to get a test program without locking, to verify that it crashes. */ #define ENABLE_LOCKING 1 /* Which tests to perform. Uncomment some of these, to verify that all tests crash if no locking is enabled. */ #define DO_TEST_LOCK 1 #define DO_TEST_RWLOCK 1 #define DO_TEST_RECURSIVE_LOCK 1 #define DO_TEST_ONCE 1 /* Whether to help the scheduler through explicit yield(). Uncomment this to see if the operating system has a fair scheduler. */ #define EXPLICIT_YIELD 1 /* Whether to print debugging messages. */ #define ENABLE_DEBUGGING 0 /* Number of simultaneous threads. */ #define THREAD_COUNT 10 /* Number of operations performed in each thread. This is quite high, because with a smaller count, say 5000, we often get an "OK" result even without ENABLE_LOCKING (on Linux/x86). */ #define REPEAT_COUNT 50000 #include #include #include #if !ENABLE_LOCKING # undef USE_POSIX_THREADS # undef USE_SOLARIS_THREADS # undef USE_PTH_THREADS # undef USE_WINDOWS_THREADS #endif #include "glthread/lock.h" #if !ENABLE_LOCKING # if TEST_POSIX_THREADS # define USE_POSIX_THREADS 1 # endif # if TEST_SOLARIS_THREADS # define USE_SOLARIS_THREADS 1 # endif # if TEST_PTH_THREADS # define USE_PTH_THREADS 1 # endif # if TEST_WINDOWS_THREADS # define USE_WINDOWS_THREADS 1 # endif #endif #include "glthread/thread.h" #include "glthread/yield.h" #if ENABLE_DEBUGGING # define dbgprintf printf #else # define dbgprintf if (0) printf #endif #if EXPLICIT_YIELD # define yield() gl_thread_yield () #else # define yield() #endif #define ACCOUNT_COUNT 4 static int account[ACCOUNT_COUNT]; static int random_account (void) { return ((unsigned int) rand () >> 3) % ACCOUNT_COUNT; } static void check_accounts (void) { int i, sum; sum = 0; for (i = 0; i < ACCOUNT_COUNT; i++) sum += account[i]; if (sum != ACCOUNT_COUNT * 1000) abort (); } /* ------------------- Test normal (non-recursive) locks ------------------- */ /* Test normal locks by having several bank accounts and several threads which shuffle around money between the accounts and another thread checking that all the money is still there. */ gl_lock_define_initialized(static, my_lock) static void * lock_mutator_thread (void *arg) { int repeat; for (repeat = REPEAT_COUNT; repeat > 0; repeat--) { int i1, i2, value; dbgprintf ("Mutator %p before lock\n", gl_thread_self_pointer ()); gl_lock_lock (my_lock); dbgprintf ("Mutator %p after lock\n", gl_thread_self_pointer ()); i1 = random_account (); i2 = random_account (); value = ((unsigned int) rand () >> 3) % 10; account[i1] += value; account[i2] -= value; dbgprintf ("Mutator %p before unlock\n", gl_thread_self_pointer ()); gl_lock_unlock (my_lock); dbgprintf ("Mutator %p after unlock\n", gl_thread_self_pointer ()); dbgprintf ("Mutator %p before check lock\n", gl_thread_self_pointer ()); gl_lock_lock (my_lock); check_accounts (); gl_lock_unlock (my_lock); dbgprintf ("Mutator %p after check unlock\n", gl_thread_self_pointer ()); yield (); } dbgprintf ("Mutator %p dying.\n", gl_thread_self_pointer ()); return NULL; } static volatile int lock_checker_done; static void * lock_checker_thread (void *arg) { while (!lock_checker_done) { dbgprintf ("Checker %p before check lock\n", gl_thread_self_pointer ()); gl_lock_lock (my_lock); check_accounts (); gl_lock_unlock (my_lock); dbgprintf ("Checker %p after check unlock\n", gl_thread_self_pointer ()); yield (); } dbgprintf ("Checker %p dying.\n", gl_thread_self_pointer ()); return NULL; } static void test_lock (void) { int i; gl_thread_t checkerthread; gl_thread_t threads[THREAD_COUNT]; /* Initialization. */ for (i = 0; i < ACCOUNT_COUNT; i++) account[i] = 1000; lock_checker_done = 0; /* Spawn the threads. */ checkerthread = gl_thread_create (lock_checker_thread, NULL); for (i = 0; i < THREAD_COUNT; i++) threads[i] = gl_thread_create (lock_mutator_thread, NULL); /* Wait for the threads to terminate. */ for (i = 0; i < THREAD_COUNT; i++) gl_thread_join (threads[i], NULL); lock_checker_done = 1; gl_thread_join (checkerthread, NULL); check_accounts (); } /* ----------------- Test read-write (non-recursive) locks ----------------- */ /* Test read-write locks by having several bank accounts and several threads which shuffle around money between the accounts and several other threads that check that all the money is still there. */ gl_rwlock_define_initialized(static, my_rwlock) static void * rwlock_mutator_thread (void *arg) { int repeat; for (repeat = REPEAT_COUNT; repeat > 0; repeat--) { int i1, i2, value; dbgprintf ("Mutator %p before wrlock\n", gl_thread_self_pointer ()); gl_rwlock_wrlock (my_rwlock); dbgprintf ("Mutator %p after wrlock\n", gl_thread_self_pointer ()); i1 = random_account (); i2 = random_account (); value = ((unsigned int) rand () >> 3) % 10; account[i1] += value; account[i2] -= value; dbgprintf ("Mutator %p before unlock\n", gl_thread_self_pointer ()); gl_rwlock_unlock (my_rwlock); dbgprintf ("Mutator %p after unlock\n", gl_thread_self_pointer ()); yield (); } dbgprintf ("Mutator %p dying.\n", gl_thread_self_pointer ()); return NULL; } static volatile int rwlock_checker_done; static void * rwlock_checker_thread (void *arg) { while (!rwlock_checker_done) { dbgprintf ("Checker %p before check rdlock\n", gl_thread_self_pointer ()); gl_rwlock_rdlock (my_rwlock); check_accounts (); gl_rwlock_unlock (my_rwlock); dbgprintf ("Checker %p after check unlock\n", gl_thread_self_pointer ()); yield (); } dbgprintf ("Checker %p dying.\n", gl_thread_self_pointer ()); return NULL; } static void test_rwlock (void) { int i; gl_thread_t checkerthreads[THREAD_COUNT]; gl_thread_t threads[THREAD_COUNT]; /* Initialization. */ for (i = 0; i < ACCOUNT_COUNT; i++) account[i] = 1000; rwlock_checker_done = 0; /* Spawn the threads. */ for (i = 0; i < THREAD_COUNT; i++) checkerthreads[i] = gl_thread_create (rwlock_checker_thread, NULL); for (i = 0; i < THREAD_COUNT; i++) threads[i] = gl_thread_create (rwlock_mutator_thread, NULL); /* Wait for the threads to terminate. */ for (i = 0; i < THREAD_COUNT; i++) gl_thread_join (threads[i], NULL); rwlock_checker_done = 1; for (i = 0; i < THREAD_COUNT; i++) gl_thread_join (checkerthreads[i], NULL); check_accounts (); } /* -------------------------- Test recursive locks -------------------------- */ /* Test recursive locks by having several bank accounts and several threads which shuffle around money between the accounts (recursively) and another thread checking that all the money is still there. */ gl_recursive_lock_define_initialized(static, my_reclock) static void recshuffle (void) { int i1, i2, value; dbgprintf ("Mutator %p before lock\n", gl_thread_self_pointer ()); gl_recursive_lock_lock (my_reclock); dbgprintf ("Mutator %p after lock\n", gl_thread_self_pointer ()); i1 = random_account (); i2 = random_account (); value = ((unsigned int) rand () >> 3) % 10; account[i1] += value; account[i2] -= value; /* Recursive with probability 0.5. */ if (((unsigned int) rand () >> 3) % 2) recshuffle (); dbgprintf ("Mutator %p before unlock\n", gl_thread_self_pointer ()); gl_recursive_lock_unlock (my_reclock); dbgprintf ("Mutator %p after unlock\n", gl_thread_self_pointer ()); } static void * reclock_mutator_thread (void *arg) { int repeat; for (repeat = REPEAT_COUNT; repeat > 0; repeat--) { recshuffle (); dbgprintf ("Mutator %p before check lock\n", gl_thread_self_pointer ()); gl_recursive_lock_lock (my_reclock); check_accounts (); gl_recursive_lock_unlock (my_reclock); dbgprintf ("Mutator %p after check unlock\n", gl_thread_self_pointer ()); yield (); } dbgprintf ("Mutator %p dying.\n", gl_thread_self_pointer ()); return NULL; } static volatile int reclock_checker_done; static void * reclock_checker_thread (void *arg) { while (!reclock_checker_done) { dbgprintf ("Checker %p before check lock\n", gl_thread_self_pointer ()); gl_recursive_lock_lock (my_reclock); check_accounts (); gl_recursive_lock_unlock (my_reclock); dbgprintf ("Checker %p after check unlock\n", gl_thread_self_pointer ()); yield (); } dbgprintf ("Checker %p dying.\n", gl_thread_self_pointer ()); return NULL; } static void test_recursive_lock (void) { int i; gl_thread_t checkerthread; gl_thread_t threads[THREAD_COUNT]; /* Initialization. */ for (i = 0; i < ACCOUNT_COUNT; i++) account[i] = 1000; reclock_checker_done = 0; /* Spawn the threads. */ checkerthread = gl_thread_create (reclock_checker_thread, NULL); for (i = 0; i < THREAD_COUNT; i++) threads[i] = gl_thread_create (reclock_mutator_thread, NULL); /* Wait for the threads to terminate. */ for (i = 0; i < THREAD_COUNT; i++) gl_thread_join (threads[i], NULL); reclock_checker_done = 1; gl_thread_join (checkerthread, NULL); check_accounts (); } /* ------------------------ Test once-only execution ------------------------ */ /* Test once-only execution by having several threads attempt to grab a once-only task simultaneously (triggered by releasing a read-write lock). */ gl_once_define(static, fresh_once) static int ready[THREAD_COUNT]; static gl_lock_t ready_lock[THREAD_COUNT]; #if ENABLE_LOCKING static gl_rwlock_t fire_signal[REPEAT_COUNT]; #else static volatile int fire_signal_state; #endif static gl_once_t once_control; static int performed; gl_lock_define_initialized(static, performed_lock) static void once_execute (void) { gl_lock_lock (performed_lock); performed++; gl_lock_unlock (performed_lock); } static void * once_contender_thread (void *arg) { int id = (int) (long) arg; int repeat; for (repeat = 0; repeat <= REPEAT_COUNT; repeat++) { /* Tell the main thread that we're ready. */ gl_lock_lock (ready_lock[id]); ready[id] = 1; gl_lock_unlock (ready_lock[id]); if (repeat == REPEAT_COUNT) break; dbgprintf ("Contender %p waiting for signal for round %d\n", gl_thread_self_pointer (), repeat); #if ENABLE_LOCKING /* Wait for the signal to go. */ gl_rwlock_rdlock (fire_signal[repeat]); /* And don't hinder the others (if the scheduler is unfair). */ gl_rwlock_unlock (fire_signal[repeat]); #else /* Wait for the signal to go. */ while (fire_signal_state <= repeat) yield (); #endif dbgprintf ("Contender %p got the signal for round %d\n", gl_thread_self_pointer (), repeat); /* Contend for execution. */ gl_once (once_control, once_execute); } return NULL; } static void test_once (void) { int i, repeat; gl_thread_t threads[THREAD_COUNT]; /* Initialize all variables. */ for (i = 0; i < THREAD_COUNT; i++) { ready[i] = 0; gl_lock_init (ready_lock[i]); } #if ENABLE_LOCKING for (i = 0; i < REPEAT_COUNT; i++) gl_rwlock_init (fire_signal[i]); #else fire_signal_state = 0; #endif /* Block all fire_signals. */ for (i = REPEAT_COUNT-1; i >= 0; i--) gl_rwlock_wrlock (fire_signal[i]); /* Spawn the threads. */ for (i = 0; i < THREAD_COUNT; i++) threads[i] = gl_thread_create (once_contender_thread, (void *) (long) i); for (repeat = 0; repeat <= REPEAT_COUNT; repeat++) { /* Wait until every thread is ready. */ dbgprintf ("Main thread before synchronizing for round %d\n", repeat); for (;;) { int ready_count = 0; for (i = 0; i < THREAD_COUNT; i++) { gl_lock_lock (ready_lock[i]); ready_count += ready[i]; gl_lock_unlock (ready_lock[i]); } if (ready_count == THREAD_COUNT) break; yield (); } dbgprintf ("Main thread after synchronizing for round %d\n", repeat); if (repeat > 0) { /* Check that exactly one thread executed the once_execute() function. */ if (performed != 1) abort (); } if (repeat == REPEAT_COUNT) break; /* Preparation for the next round: Initialize once_control. */ memcpy (&once_control, &fresh_once, sizeof (gl_once_t)); /* Preparation for the next round: Reset the performed counter. */ performed = 0; /* Preparation for the next round: Reset the ready flags. */ for (i = 0; i < THREAD_COUNT; i++) { gl_lock_lock (ready_lock[i]); ready[i] = 0; gl_lock_unlock (ready_lock[i]); } /* Signal all threads simultaneously. */ dbgprintf ("Main thread giving signal for round %d\n", repeat); #if ENABLE_LOCKING gl_rwlock_unlock (fire_signal[repeat]); #else fire_signal_state = repeat + 1; #endif } /* Wait for the threads to terminate. */ for (i = 0; i < THREAD_COUNT; i++) gl_thread_join (threads[i], NULL); } /* -------------------------------------------------------------------------- */ int main () { #if TEST_PTH_THREADS if (!pth_init ()) abort (); #endif #if DO_TEST_LOCK printf ("Starting test_lock ..."); fflush (stdout); test_lock (); printf (" OK\n"); fflush (stdout); #endif #if DO_TEST_RWLOCK printf ("Starting test_rwlock ..."); fflush (stdout); test_rwlock (); printf (" OK\n"); fflush (stdout); #endif #if DO_TEST_RECURSIVE_LOCK printf ("Starting test_recursive_lock ..."); fflush (stdout); test_recursive_lock (); printf (" OK\n"); fflush (stdout); #endif #if DO_TEST_ONCE printf ("Starting test_once ..."); fflush (stdout); test_once (); printf (" OK\n"); fflush (stdout); #endif return 0; } #else /* No multithreading available. */ #include int main () { fputs ("Skipping test: multithreading not enabled\n", stderr); return 77; } #endif gnuastro-0.2.33-8a3b/bootstrapped/tests/test-localename.c0000644000175000017500000005446313004436755020231 00000000000000/* Test of gl_locale_name function and its variants. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include "localename.h" #include #include #include #include "macros.h" #if HAVE_NEWLOCALE static struct { int cat; int mask; const char *string; } const categories[] = { { LC_CTYPE, LC_CTYPE_MASK, "LC_CTYPE" }, { LC_NUMERIC, LC_NUMERIC_MASK, "LC_NUMERIC" }, { LC_TIME, LC_TIME_MASK, "LC_TIME" }, { LC_COLLATE, LC_COLLATE_MASK, "LC_COLLATE" }, { LC_MONETARY, LC_MONETARY_MASK, "LC_MONETARY" }, { LC_MESSAGES, LC_MESSAGES_MASK, "LC_MESSAGES" } # ifdef LC_PAPER , { LC_PAPER, LC_PAPER_MASK, "LC_PAPER" } # endif # ifdef LC_NAME , { LC_NAME, LC_NAME_MASK, "LC_NAME" } # endif # ifdef LC_ADDRESS , { LC_ADDRESS, LC_ADDRESS_MASK, "LC_ADDRESS" } # endif # ifdef LC_TELEPHONE , { LC_TELEPHONE, LC_TELEPHONE_MASK, "LC_TELEPHONE" } # endif # ifdef LC_MEASUREMENT , { LC_MEASUREMENT, LC_MEASUREMENT_MASK, "LC_MEASUREMENT" } # endif # ifdef LC_IDENTIFICATION , { LC_IDENTIFICATION, LC_IDENTIFICATION_MASK, "LC_IDENTIFICATION" } # endif }; #endif /* Test the gl_locale_name() function. */ static void test_locale_name (void) { const char *name; /* Check that gl_locale_name returns non-NULL. */ ASSERT (gl_locale_name (LC_MESSAGES, "LC_MESSAGES") != NULL); /* Get into a defined state, */ setlocale (LC_ALL, "en_US.UTF-8"); #if HAVE_NEWLOCALE uselocale (LC_GLOBAL_LOCALE); #endif /* Check that when all environment variables are unset, gl_locale_name returns the default locale. */ unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LC_NUMERIC"); unsetenv ("LANG"); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), gl_locale_name_default ()) == 0); ASSERT (strcmp (gl_locale_name (LC_NUMERIC, "LC_NUMERIC"), gl_locale_name_default ()) == 0); /* Check that an empty environment variable is treated like an unset environment variable. */ setenv ("LC_ALL", "", 1); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), gl_locale_name_default ()) == 0); unsetenv ("LC_ALL"); setenv ("LC_CTYPE", "", 1); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), gl_locale_name_default ()) == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "", 1); unsetenv ("LANG"); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), gl_locale_name_default ()) == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "", 1); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), gl_locale_name_default ()) == 0); /* Check that LC_ALL overrides the others, and LANG is overridden by the others. */ setenv ("LC_ALL", "C", 1); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), "C") == 0); unsetenv ("LC_ALL"); setenv ("LC_CTYPE", "C", 1); setenv ("LC_MESSAGES", "C", 1); unsetenv ("LANG"); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), "C") == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "C", 1); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), "C") == 0); /* Check mixed situations. */ unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "fr_FR.UTF-8", 1); setenv ("LANG", "de_DE.UTF-8", 1); if (setlocale (LC_ALL, "") != NULL) { name = gl_locale_name (LC_CTYPE, "LC_CTYPE"); ASSERT (strcmp (name, "de_DE.UTF-8") == 0); name = gl_locale_name (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); } unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "fr_FR.UTF-8", 1); unsetenv ("LANG"); if (setlocale (LC_ALL, "") != NULL) { name = gl_locale_name (LC_CTYPE, "LC_CTYPE"); ASSERT (strcmp (name, gl_locale_name_default ()) == 0); name = gl_locale_name (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); } #if HAVE_NEWLOCALE /* Check that gl_locale_name considers the thread locale. */ { locale_t locale = newlocale (LC_ALL_MASK, "fr_FR.UTF-8", NULL); if (locale != NULL) { uselocale (locale); name = gl_locale_name (LC_CTYPE, "LC_CTYPE"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); name = gl_locale_name (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } /* Check that gl_locale_name distinguishes different categories of the thread locale, and that the name is the right one for each. */ { unsigned int i; for (i = 0; i < SIZEOF (categories); i++) { int category_mask = categories[i].mask; locale_t loc = newlocale (LC_ALL_MASK, "fr_FR.UTF-8", NULL); if (loc != NULL) { locale_t locale = newlocale (category_mask, "de_DE.UTF-8", loc); if (locale == NULL) freelocale (loc); else { unsigned int j; uselocale (locale); for (j = 0; j < SIZEOF (categories); j++) { const char *name_j = gl_locale_name (categories[j].cat, categories[j].string); if (j == i) ASSERT (strcmp (name_j, "de_DE.UTF-8") == 0); else ASSERT (strcmp (name_j, "fr_FR.UTF-8") == 0); } uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } } } #endif } /* Test the gl_locale_name_thread() function. */ static void test_locale_name_thread (void) { /* Get into a defined state, */ setlocale (LC_ALL, "en_US.UTF-8"); #if HAVE_NEWLOCALE /* Check that gl_locale_name_thread returns NULL when no thread locale is set. */ uselocale (LC_GLOBAL_LOCALE); ASSERT (gl_locale_name_thread (LC_CTYPE, "LC_CTYPE") == NULL); ASSERT (gl_locale_name_thread (LC_MESSAGES, "LC_MESSAGES") == NULL); /* Check that gl_locale_name_thread considers the thread locale. */ { locale_t locale = newlocale (LC_ALL_MASK, "fr_FR.UTF-8", NULL); if (locale != NULL) { const char *name; uselocale (locale); name = gl_locale_name_thread (LC_CTYPE, "LC_CTYPE"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); name = gl_locale_name_thread (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } /* Check that gl_locale_name_thread distinguishes different categories of the thread locale, and that the name is the right one for each. */ { unsigned int i; for (i = 0; i < SIZEOF (categories); i++) { int category_mask = categories[i].mask; locale_t loc = newlocale (LC_ALL_MASK, "fr_FR.UTF-8", NULL); if (loc != NULL) { locale_t locale = newlocale (category_mask, "de_DE.UTF-8", loc); if (locale == NULL) freelocale (loc); else { unsigned int j; uselocale (locale); for (j = 0; j < SIZEOF (categories); j++) { const char *name_j = gl_locale_name_thread (categories[j].cat, categories[j].string); if (j == i) ASSERT (strcmp (name_j, "de_DE.UTF-8") == 0); else ASSERT (strcmp (name_j, "fr_FR.UTF-8") == 0); } uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } } } /* Check that gl_locale_name_thread returns a string that is allocated with indefinite extent. */ { /* Try many locale names in turn, in order to defeat possible caches. */ static const char * const choices[] = { "C", "POSIX", "af_ZA", "af_ZA.UTF-8", "am_ET", "am_ET.UTF-8", "be_BY", "be_BY.UTF-8", "bg_BG", "bg_BG.UTF-8", "ca_ES", "ca_ES.UTF-8", "cs_CZ", "cs_CZ.UTF-8", "da_DK", "da_DK.UTF-8", "de_AT", "de_AT.UTF-8", "de_CH", "de_CH.UTF-8", "de_DE", "de_DE.UTF-8", "el_GR", "el_GR.UTF-8", "en_AU", "en_AU.UTF-8", "en_CA", "en_CA.UTF-8", "en_GB", "en_GB.UTF-8", "en_IE", "en_IE.UTF-8", "en_NZ", "en_NZ.UTF-8", "en_US", "en_US.UTF-8", "es_ES", "es_ES.UTF-8", "et_EE", "et_EE.UTF-8", "eu_ES", "eu_ES.UTF-8", "fi_FI", "fi_FI.UTF-8", "fr_BE", "fr_BE.UTF-8", "fr_CA", "fr_CA.UTF-8", "fr_CH", "fr_CH.UTF-8", "fr_FR", "fr_FR.UTF-8", "he_IL", "he_IL.UTF-8", "hr_HR", "hr_HR.UTF-8", "hu_HU", "hu_HU.UTF-8", "hy_AM", "is_IS", "is_IS.UTF-8", "it_CH", "it_CH.UTF-8", "it_IT", "it_IT.UTF-8", "ja_JP.UTF-8", "kk_KZ", "kk_KZ.UTF-8", "ko_KR.UTF-8", "lt_LT", "lt_LT.UTF-8", "nl_BE", "nl_BE.UTF-8", "nl_NL", "nl_NL.UTF-8", "no_NO", "no_NO.UTF-8", "pl_PL", "pl_PL.UTF-8", "pt_BR", "pt_BR.UTF-8", "pt_PT", "pt_PT.UTF-8", "ro_RO", "ro_RO.UTF-8", "ru_RU", "ru_RU.UTF-8", "sk_SK", "sk_SK.UTF-8", "sl_SI", "sl_SI.UTF-8", "sv_SE", "sv_SE.UTF-8", "tr_TR", "tr_TR.UTF-8", "uk_UA", "uk_UA.UTF-8", "zh_CN", "zh_CN.UTF-8", "zh_HK", "zh_HK.UTF-8", "zh_TW", "zh_TW.UTF-8" }; /* Remember which locales are available. */ unsigned char /* bool */ available[SIZEOF (choices)]; /* Array of remembered results of gl_locale_name_thread. */ const char *unsaved_names[SIZEOF (choices)][SIZEOF (categories)]; /* Array of remembered results of gl_locale_name_thread, stored in safe memory. */ char *saved_names[SIZEOF (choices)][SIZEOF (categories)]; unsigned int j; for (j = 0; j < SIZEOF (choices); j++) { locale_t locale = newlocale (LC_ALL_MASK, choices[j], NULL); available[j] = (locale != NULL); if (locale != NULL) { unsigned int i; uselocale (locale); for (i = 0; i < SIZEOF (categories); i++) { unsaved_names[j][i] = gl_locale_name_thread (categories[i].cat, categories[i].string); saved_names[j][i] = strdup (unsaved_names[j][i]); } uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } /* Verify the unsaved_names are still valid. */ for (j = 0; j < SIZEOF (choices); j++) if (available[j]) { unsigned int i; for (i = 0; i < SIZEOF (categories); i++) ASSERT (strcmp (unsaved_names[j][i], saved_names[j][i]) == 0); } /* Allocate many locales, without freeing them. This is an attempt at overwriting as much of the previously allocated memory as possible. */ for (j = SIZEOF (choices); j > 0; ) { j--; if (available[j]) { locale_t locale = newlocale (LC_ALL_MASK, choices[j], NULL); unsigned int i; ASSERT (locale != NULL); uselocale (locale); for (i = 0; i < SIZEOF (categories); i++) { const char *name = gl_locale_name_thread (categories[i].cat, categories[i].string); ASSERT (strcmp (unsaved_names[j][i], name) == 0); } uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } /* Verify the unsaved_names are still valid. */ for (j = 0; j < SIZEOF (choices); j++) if (available[j]) { unsigned int i; for (i = 0; i < SIZEOF (categories); i++) { ASSERT (strcmp (unsaved_names[j][i], saved_names[j][i]) == 0); free (saved_names[j][i]); } } } #else /* Check that gl_locale_name_thread always returns NULL. */ ASSERT (gl_locale_name_thread (LC_CTYPE, "LC_CTYPE") == NULL); ASSERT (gl_locale_name_thread (LC_MESSAGES, "LC_MESSAGES") == NULL); #endif } /* Test the gl_locale_name_posix() function. */ static void test_locale_name_posix (void) { const char *name; /* Get into a defined state, */ setlocale (LC_ALL, "en_US.UTF-8"); #if HAVE_NEWLOCALE uselocale (LC_GLOBAL_LOCALE); #endif /* Check that when all environment variables are unset, gl_locale_name_posix returns either NULL or the default locale. */ unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LC_NUMERIC"); unsetenv ("LANG"); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (name == NULL || strcmp (name, gl_locale_name_default ()) == 0); name = gl_locale_name_posix (LC_NUMERIC, "LC_NUMERIC"); ASSERT (name == NULL || strcmp (name, gl_locale_name_default ()) == 0); /* Check that an empty environment variable is treated like an unset environment variable. */ setenv ("LC_ALL", "", 1); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (name == NULL || strcmp (name, gl_locale_name_default ()) == 0); unsetenv ("LC_ALL"); setenv ("LC_CTYPE", "", 1); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (name == NULL || strcmp (name, gl_locale_name_default ()) == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "", 1); unsetenv ("LANG"); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (name == NULL || strcmp (name, gl_locale_name_default ()) == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "", 1); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (name == NULL || strcmp (name, gl_locale_name_default ()) == 0); /* Check that LC_ALL overrides the others, and LANG is overridden by the others. */ setenv ("LC_ALL", "C", 1); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); unsetenv ("LC_ALL"); setenv ("LC_CTYPE", "C", 1); setenv ("LC_MESSAGES", "C", 1); unsetenv ("LANG"); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "C", 1); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); /* Check mixed situations. */ unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "fr_FR.UTF-8", 1); setenv ("LANG", "de_DE.UTF-8", 1); if (setlocale (LC_ALL, "") != NULL) { name = gl_locale_name_posix (LC_CTYPE, "LC_CTYPE"); ASSERT (strcmp (name, "de_DE.UTF-8") == 0); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); } unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "fr_FR.UTF-8", 1); unsetenv ("LANG"); if (setlocale (LC_ALL, "") != NULL) { name = gl_locale_name_posix (LC_CTYPE, "LC_CTYPE"); ASSERT (name == NULL || strcmp (name, gl_locale_name_default ()) == 0); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); } #if HAVE_NEWLOCALE /* Check that gl_locale_name_posix ignores the thread locale. */ { locale_t locale = newlocale (LC_ALL_MASK, "fr_FR.UTF-8", NULL); if (locale != NULL) { unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "C", 1); setlocale (LC_ALL, ""); uselocale (locale); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } #endif } /* Test the gl_locale_name_environ() function. */ static void test_locale_name_environ (void) { const char *name; /* Get into a defined state, */ setlocale (LC_ALL, "en_US.UTF-8"); #if HAVE_NEWLOCALE uselocale (LC_GLOBAL_LOCALE); #endif /* Check that when all environment variables are unset, gl_locale_name_environ returns NULL. */ unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LC_NUMERIC"); unsetenv ("LANG"); ASSERT (gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES") == NULL); ASSERT (gl_locale_name_environ (LC_NUMERIC, "LC_NUMERIC") == NULL); /* Check that an empty environment variable is treated like an unset environment variable. */ setenv ("LC_ALL", "", 1); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); ASSERT (gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES") == NULL); unsetenv ("LC_ALL"); setenv ("LC_CTYPE", "", 1); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); ASSERT (gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES") == NULL); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "", 1); unsetenv ("LANG"); ASSERT (gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES") == NULL); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "", 1); ASSERT (gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES") == NULL); /* Check that LC_ALL overrides the others, and LANG is overridden by the others. */ setenv ("LC_ALL", "C", 1); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); name = gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); unsetenv ("LC_ALL"); setenv ("LC_CTYPE", "C", 1); setenv ("LC_MESSAGES", "C", 1); unsetenv ("LANG"); name = gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "C", 1); name = gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); /* Check mixed situations. */ unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "fr_FR.UTF-8", 1); setenv ("LANG", "de_DE.UTF-8", 1); name = gl_locale_name_environ (LC_CTYPE, "LC_CTYPE"); ASSERT (strcmp (name, "de_DE.UTF-8") == 0); name = gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "fr_FR.UTF-8", 1); unsetenv ("LANG"); name = gl_locale_name_environ (LC_CTYPE, "LC_CTYPE"); ASSERT (name == NULL); name = gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); #if HAVE_NEWLOCALE /* Check that gl_locale_name_environ ignores the thread locale. */ { locale_t locale = newlocale (LC_ALL_MASK, "fr_FR.UTF-8", NULL); if (locale != NULL) { unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "C", 1); setlocale (LC_ALL, ""); uselocale (locale); name = gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } #endif } /* Test the gl_locale_name_default() function. */ static void test_locale_name_default (void) { const char *name = gl_locale_name_default (); ASSERT (name != NULL); /* Only Mac OS X and Windows have a facility for the user to set the default locale. */ #if !((defined __APPLE__ && defined __MACH__) || (defined _WIN32 || defined __WIN32__ || defined __CYGWIN__)) ASSERT (strcmp (name, "C") == 0); #endif #if HAVE_NEWLOCALE /* Check that gl_locale_name_default ignores the thread locale. */ { locale_t locale = newlocale (LC_ALL_MASK, "fr_FR.UTF-8", NULL); if (locale != NULL) { uselocale (locale); ASSERT (strcmp (gl_locale_name_default (), name) == 0); uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } #endif } int main () { test_locale_name (); test_locale_name_thread (); test_locale_name_posix (); test_locale_name_environ (); test_locale_name_default (); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-localeconv.c0000644000175000017500000000433713004436755020251 00000000000000/* Test of localeconv() function. Copyright (C) 2012-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2012. */ #include #include #include "signature.h" SIGNATURE_CHECK (localeconv, struct lconv *, (void)); #include #include #include "macros.h" int main () { /* Test localeconv() result in the "C" locale. */ { struct lconv *l = localeconv (); ASSERT (STREQ (l->decimal_point, ".")); ASSERT (STREQ (l->thousands_sep, "")); #if !(defined __FreeBSD__ || defined __sun) ASSERT (STREQ (l->grouping, "")); #endif ASSERT (STREQ (l->mon_decimal_point, "")); ASSERT (STREQ (l->mon_thousands_sep, "")); #if !(defined __FreeBSD__ || defined __sun) ASSERT (STREQ (l->mon_grouping, "")); #endif ASSERT (STREQ (l->positive_sign, "")); ASSERT (STREQ (l->negative_sign, "")); ASSERT (STREQ (l->currency_symbol, "")); ASSERT (l->frac_digits == CHAR_MAX); ASSERT (l->p_cs_precedes == CHAR_MAX); ASSERT (l->p_sign_posn == CHAR_MAX); ASSERT (l->p_sep_by_space == CHAR_MAX); ASSERT (l->n_cs_precedes == CHAR_MAX); ASSERT (l->n_sign_posn == CHAR_MAX); ASSERT (l->n_sep_by_space == CHAR_MAX); ASSERT (STREQ (l->int_curr_symbol, "")); ASSERT (l->int_frac_digits == CHAR_MAX); ASSERT (l->int_p_cs_precedes == CHAR_MAX); ASSERT (l->int_p_sign_posn == CHAR_MAX); ASSERT (l->int_p_sep_by_space == CHAR_MAX); ASSERT (l->int_n_cs_precedes == CHAR_MAX); ASSERT (l->int_n_sign_posn == CHAR_MAX); ASSERT (l->int_n_sep_by_space == CHAR_MAX); } return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-locale.c0000644000175000017500000000441313004436755017356 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" int a[] = { LC_ALL, LC_COLLATE, LC_CTYPE, LC_MESSAGES, LC_MONETARY, LC_NUMERIC, LC_TIME }; /* Check that the 'struct lconv' type is defined. */ struct lconv l; int ls; /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); int main () { #if HAVE_NEWLOCALE /* Check that the locale_t type and the LC_GLOBAL_LOCALE macro are defined. */ locale_t b = LC_GLOBAL_LOCALE; (void) b; #endif /* Check that 'struct lconv' has the ISO C and POSIX specified members. */ ls += sizeof (*l.decimal_point); ls += sizeof (*l.thousands_sep); ls += sizeof (*l.grouping); ls += sizeof (*l.mon_decimal_point); ls += sizeof (*l.mon_thousands_sep); ls += sizeof (*l.mon_grouping); ls += sizeof (*l.positive_sign); ls += sizeof (*l.negative_sign); ls += sizeof (*l.currency_symbol); ls += sizeof (l.frac_digits); ls += sizeof (l.p_cs_precedes); ls += sizeof (l.p_sign_posn); ls += sizeof (l.p_sep_by_space); ls += sizeof (l.n_cs_precedes); ls += sizeof (l.n_sign_posn); ls += sizeof (l.n_sep_by_space); ls += sizeof (*l.int_curr_symbol); ls += sizeof (l.int_frac_digits); ls += sizeof (l.int_p_cs_precedes); ls += sizeof (l.int_p_sign_posn); ls += sizeof (l.int_p_sep_by_space); ls += sizeof (l.int_n_cs_precedes); ls += sizeof (l.int_n_sign_posn); ls += sizeof (l.int_n_sep_by_space); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-limits-h.c0000644000175000017500000000310513004436755017642 00000000000000/* Test of substitute. Copyright 2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paul Eggert. */ #include #include #include "verify.h" #if 4 < __GNUC__ + (3 <= __GNUC_MINOR__) # pragma GCC diagnostic ignored "-Woverlength-strings" #endif /* Macros specified by ISO/IEC TS 18661-1:2014. */ #define verify_width(width, min, max) \ verify ((max) >> ((width) - 1 - ((min) < 0)) == 1) verify_width (CHAR_WIDTH, CHAR_MIN, CHAR_MAX); verify_width (SCHAR_WIDTH, SCHAR_MIN, SCHAR_MAX); verify_width (UCHAR_WIDTH, 0, UCHAR_MAX); verify_width (SHRT_WIDTH, SHRT_MIN, SHRT_MAX); verify_width (USHRT_WIDTH, 0, USHRT_MAX); verify_width (INT_WIDTH, INT_MIN, INT_MAX); verify_width (UINT_WIDTH, 0, UINT_MAX); verify_width (LONG_WIDTH, LONG_MIN, LONG_MAX); verify_width (ULONG_WIDTH, 0, ULONG_MAX); verify_width (LLONG_WIDTH, LLONG_MIN, LLONG_MAX); verify_width (ULLONG_WIDTH, 0, ULLONG_MAX); int main (void) { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-langinfo.c0000644000175000017500000000357113004436755017720 00000000000000/* Test of substitute. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ #include #include /* Check that all the nl_item values are defined. */ int items[] = { /* nl_langinfo items of the LC_CTYPE category */ CODESET, /* nl_langinfo items of the LC_NUMERIC category */ RADIXCHAR, THOUSEP, /* nl_langinfo items of the LC_TIME category */ D_T_FMT, D_FMT, T_FMT, T_FMT_AMPM, AM_STR, PM_STR, DAY_1, DAY_2, DAY_3, DAY_4, DAY_5, DAY_6, DAY_7, ABDAY_1, ABDAY_2, ABDAY_3, ABDAY_4, ABDAY_5, ABDAY_6, ABDAY_7, MON_1, MON_2, MON_3, MON_4, MON_5, MON_6, MON_7, MON_8, MON_9, MON_10, MON_11, MON_12, ABMON_1, ABMON_2, ABMON_3, ABMON_4, ABMON_5, ABMON_6, ABMON_7, ABMON_8, ABMON_9, ABMON_10, ABMON_11, ABMON_12, ERA, ERA_D_FMT, ERA_D_T_FMT, ERA_T_FMT, ALT_DIGITS, /* nl_langinfo items of the LC_MONETARY category */ CRNCYSTR, /* nl_langinfo items of the LC_MESSAGES category */ YESEXPR, NOEXPR }; int main (void) { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-inttypes.c0000644000175000017500000000606013004436755017776 00000000000000/* Test of substitute. Copyright (C) 2006-2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include /* Tests for macros supposed to be defined in inttypes.h. */ const char *k = /* implicit string concatenation */ #ifdef INT8_MAX PRId8 PRIi8 #endif #ifdef UINT8_MAX PRIo8 PRIu8 PRIx8 PRIX8 #endif #ifdef INT16_MAX PRId16 PRIi16 #endif #ifdef UINT16_MAX PRIo16 PRIu16 PRIx16 PRIX16 #endif #ifdef INT32_MAX PRId32 PRIi32 #endif #ifdef UINT32_MAX PRIo32 PRIu32 PRIx32 PRIX32 #endif #ifdef INT64_MAX PRId64 PRIi64 #endif #ifdef UINT64_MAX PRIo64 PRIu64 PRIx64 PRIX64 #endif PRIdLEAST8 PRIiLEAST8 PRIoLEAST8 PRIuLEAST8 PRIxLEAST8 PRIXLEAST8 PRIdLEAST16 PRIiLEAST16 PRIoLEAST16 PRIuLEAST16 PRIxLEAST16 PRIXLEAST16 PRIdLEAST32 PRIiLEAST32 PRIoLEAST32 PRIuLEAST32 PRIxLEAST32 PRIXLEAST32 PRIdLEAST64 PRIiLEAST64 PRIoLEAST64 PRIuLEAST64 PRIxLEAST64 PRIXLEAST64 PRIdFAST8 PRIiFAST8 PRIoFAST8 PRIuFAST8 PRIxFAST8 PRIXFAST8 PRIdFAST16 PRIiFAST16 PRIoFAST16 PRIuFAST16 PRIxFAST16 PRIXFAST16 PRIdFAST32 PRIiFAST32 PRIoFAST32 PRIuFAST32 PRIxFAST32 PRIXFAST32 PRIdFAST64 PRIiFAST64 PRIoFAST64 PRIuFAST64 PRIxFAST64 PRIXFAST64 PRIdMAX PRIiMAX PRIoMAX PRIuMAX PRIxMAX PRIXMAX #ifdef INTPTR_MAX PRIdPTR PRIiPTR #endif #ifdef UINTPTR_MAX PRIoPTR PRIuPTR PRIxPTR PRIXPTR #endif ; const char *l = /* implicit string concatenation */ #ifdef INT8_MAX SCNd8 SCNi8 #endif #ifdef UINT8_MAX SCNo8 SCNu8 SCNx8 #endif #ifdef INT16_MAX SCNd16 SCNi16 #endif #ifdef UINT16_MAX SCNo16 SCNu16 SCNx16 #endif #ifdef INT32_MAX SCNd32 SCNi32 #endif #ifdef UINT32_MAX SCNo32 SCNu32 SCNx32 #endif #ifdef INT64_MAX SCNd64 SCNi64 #endif #ifdef UINT64_MAX SCNo64 SCNu64 SCNx64 #endif SCNdLEAST8 SCNiLEAST8 SCNoLEAST8 SCNuLEAST8 SCNxLEAST8 SCNdLEAST16 SCNiLEAST16 SCNoLEAST16 SCNuLEAST16 SCNxLEAST16 SCNdLEAST32 SCNiLEAST32 SCNoLEAST32 SCNuLEAST32 SCNxLEAST32 SCNdLEAST64 SCNiLEAST64 SCNoLEAST64 SCNuLEAST64 SCNxLEAST64 SCNdFAST8 SCNiFAST8 SCNoFAST8 SCNuFAST8 SCNxFAST8 SCNdFAST16 SCNiFAST16 SCNoFAST16 SCNuFAST16 SCNxFAST16 SCNdFAST32 SCNiFAST32 SCNoFAST32 SCNuFAST32 SCNxFAST32 SCNdFAST64 SCNiFAST64 SCNoFAST64 SCNuFAST64 SCNxFAST64 SCNdMAX SCNiMAX SCNoMAX SCNuMAX SCNxMAX #ifdef INTPTR_MAX SCNdPTR SCNiPTR #endif #ifdef UINTPTR_MAX SCNoPTR SCNuPTR SCNxPTR #endif ; int main (void) { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-intprops.c0000644000175000017500000004177213004436755020006 00000000000000/* Test intprops.h. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paul Eggert. */ /* Tell gcc not to warn about the long expressions that the overflow macros expand to, or about the (X < 0) expressions. */ #if 4 < __GNUC__ + (3 <= __GNUC_MINOR__) # pragma GCC diagnostic ignored "-Woverlength-strings" # pragma GCC diagnostic ignored "-Wtype-limits" /* Work around a bug in GCC 6.1 and earlier; see: https://gcc.gnu.org/bugzilla/show_bug.cgi?id=68971 */ # pragma GCC diagnostic ignored "-Woverflow" #endif #include #include "intprops.h" #include "verify.h" #include #include #include #include "macros.h" /* VERIFY (X) uses a static assertion for compilers that are known to work, and falls back on a dynamic assertion for other compilers. These tests should be checkable via 'verify' rather than 'ASSERT', but using 'verify' would run into a bug with HP-UX 11.23 cc; see . */ #if __GNUC__ || __SUNPRO_C # define VERIFY(x) do { verify (x); } while (0) #else # define VERIFY(x) ASSERT (x) #endif #define DONTCARE __LINE__ int main (void) { /* Use VERIFY for tests that must be integer constant expressions, ASSERT otherwise. */ /* TYPE_IS_INTEGER. */ ASSERT (TYPE_IS_INTEGER (bool)); ASSERT (TYPE_IS_INTEGER (char)); ASSERT (TYPE_IS_INTEGER (signed char)); ASSERT (TYPE_IS_INTEGER (unsigned char)); ASSERT (TYPE_IS_INTEGER (short int)); ASSERT (TYPE_IS_INTEGER (unsigned short int)); ASSERT (TYPE_IS_INTEGER (int)); ASSERT (TYPE_IS_INTEGER (unsigned int)); ASSERT (TYPE_IS_INTEGER (long int)); ASSERT (TYPE_IS_INTEGER (unsigned long int)); ASSERT (TYPE_IS_INTEGER (intmax_t)); ASSERT (TYPE_IS_INTEGER (uintmax_t)); ASSERT (! TYPE_IS_INTEGER (float)); ASSERT (! TYPE_IS_INTEGER (double)); ASSERT (! TYPE_IS_INTEGER (long double)); /* TYPE_SIGNED. */ /* VERIFY (! TYPE_SIGNED (bool)); // not guaranteed by gnulib substitute */ VERIFY (TYPE_SIGNED (signed char)); VERIFY (! TYPE_SIGNED (unsigned char)); VERIFY (TYPE_SIGNED (short int)); VERIFY (! TYPE_SIGNED (unsigned short int)); VERIFY (TYPE_SIGNED (int)); VERIFY (! TYPE_SIGNED (unsigned int)); VERIFY (TYPE_SIGNED (long int)); VERIFY (! TYPE_SIGNED (unsigned long int)); VERIFY (TYPE_SIGNED (intmax_t)); VERIFY (! TYPE_SIGNED (uintmax_t)); ASSERT (TYPE_SIGNED (float)); ASSERT (TYPE_SIGNED (double)); ASSERT (TYPE_SIGNED (long double)); /* Integer representation. Check that it is two's complement. */ VERIFY (INT_MIN + INT_MAX < 0); /* TYPE_MINIMUM, TYPE_MAXIMUM. */ VERIFY (TYPE_MINIMUM (char) == CHAR_MIN); VERIFY (TYPE_MAXIMUM (char) == CHAR_MAX); VERIFY (TYPE_MINIMUM (unsigned char) == 0); VERIFY (TYPE_MAXIMUM (unsigned char) == UCHAR_MAX); VERIFY (TYPE_MINIMUM (signed char) == SCHAR_MIN); VERIFY (TYPE_MAXIMUM (signed char) == SCHAR_MAX); VERIFY (TYPE_MINIMUM (short int) == SHRT_MIN); VERIFY (TYPE_MAXIMUM (short int) == SHRT_MAX); VERIFY (TYPE_MINIMUM (unsigned short int) == 0); VERIFY (TYPE_MAXIMUM (unsigned short int) == USHRT_MAX); VERIFY (TYPE_MINIMUM (int) == INT_MIN); VERIFY (TYPE_MAXIMUM (int) == INT_MAX); VERIFY (TYPE_MINIMUM (unsigned int) == 0); VERIFY (TYPE_MAXIMUM (unsigned int) == UINT_MAX); VERIFY (TYPE_MINIMUM (long int) == LONG_MIN); VERIFY (TYPE_MAXIMUM (long int) == LONG_MAX); VERIFY (TYPE_MINIMUM (unsigned long int) == 0); VERIFY (TYPE_MAXIMUM (unsigned long int) == ULONG_MAX); VERIFY (TYPE_MINIMUM (intmax_t) == INTMAX_MIN); VERIFY (TYPE_MAXIMUM (intmax_t) == INTMAX_MAX); VERIFY (TYPE_MINIMUM (uintmax_t) == 0); VERIFY (TYPE_MAXIMUM (uintmax_t) == UINTMAX_MAX); /* INT_BITS_STRLEN_BOUND. */ VERIFY (INT_BITS_STRLEN_BOUND (1) == 1); VERIFY (INT_BITS_STRLEN_BOUND (2620) == 789); /* INT_STRLEN_BOUND, INT_BUFSIZE_BOUND. */ #ifdef INT32_MAX /* POSIX guarantees int32_t; this ports to non-POSIX. */ VERIFY (INT_STRLEN_BOUND (int32_t) == sizeof ("-2147483648") - 1); VERIFY (INT_BUFSIZE_BOUND (int32_t) == sizeof ("-2147483648")); #endif #ifdef INT64_MAX VERIFY (INT_STRLEN_BOUND (int64_t) == sizeof ("-9223372036854775808") - 1); VERIFY (INT_BUFSIZE_BOUND (int64_t) == sizeof ("-9223372036854775808")); #endif /* All the INT__RANGE_OVERFLOW tests are equally valid as INT__OVERFLOW tests, so define macros to do both. OP is the operation, OPNAME its symbolic name, A and B its operands, T the result type, V the overflow flag, and VRES the result if V and if two's complement. CHECK_BINOP is for most binary operatinos, CHECK_SBINOP for binary +, -, * when the result type is signed, and CHECK_UNOP for unary operations. */ #define CHECK_BINOP(op, opname, a, b, t, v, vres) \ VERIFY (INT_##opname##_RANGE_OVERFLOW (a, b, TYPE_MINIMUM (t), \ TYPE_MAXIMUM (t)) \ == (v)); \ VERIFY (INT_##opname##_OVERFLOW (a, b) == (v)) #define CHECK_SBINOP(op, opname, a, b, t, v, vres) \ CHECK_BINOP(op, opname, a, b, t, v, vres); \ { \ t result; \ ASSERT (INT_##opname##_WRAPV (a, b, &result) == (v)); \ ASSERT (result == ((v) ? (vres) : ((a) op (b)))); \ } #define CHECK_UNOP(op, opname, a, t, v) \ VERIFY (INT_##opname##_RANGE_OVERFLOW (a, TYPE_MINIMUM (t), \ TYPE_MAXIMUM (t)) \ == (v)); \ VERIFY (INT_##opname##_OVERFLOW (a) == (v)) /* INT__RANGE_OVERFLOW, INT__OVERFLOW. */ VERIFY (INT_ADD_RANGE_OVERFLOW (INT_MAX, 1, INT_MIN, INT_MAX)); VERIFY (INT_ADD_OVERFLOW (INT_MAX, 1)); CHECK_SBINOP (+, ADD, INT_MAX, 1, int, true, INT_MIN); CHECK_SBINOP (+, ADD, INT_MAX, -1, int, false, INT_MAX - 1); CHECK_SBINOP (+, ADD, INT_MIN, 1, int, false, INT_MIN + 1); CHECK_SBINOP (+, ADD, INT_MIN, -1, int, true, INT_MAX); CHECK_BINOP (+, ADD, UINT_MAX, 1u, unsigned int, true, 0u); CHECK_BINOP (+, ADD, 0u, 1u, unsigned int, false, 1u); CHECK_SBINOP (-, SUBTRACT, INT_MAX, 1, int, false, INT_MAX - 1); CHECK_SBINOP (-, SUBTRACT, INT_MAX, -1, int, true, INT_MIN); CHECK_SBINOP (-, SUBTRACT, INT_MIN, 1, int, true, INT_MAX); CHECK_SBINOP (-, SUBTRACT, INT_MIN, -1, int, false, INT_MIN - -1); CHECK_BINOP (-, SUBTRACT, UINT_MAX, 1u, unsigned int, false, UINT_MAX - 1u); CHECK_BINOP (-, SUBTRACT, 0u, 1u, unsigned int, true, 0u - 1u); CHECK_UNOP (-, NEGATE, INT_MIN, int, true); CHECK_UNOP (-, NEGATE, 0, int, false); CHECK_UNOP (-, NEGATE, INT_MAX, int, false); CHECK_UNOP (-, NEGATE, 0u, unsigned int, false); CHECK_UNOP (-, NEGATE, 1u, unsigned int, true); CHECK_UNOP (-, NEGATE, UINT_MAX, unsigned int, true); CHECK_SBINOP (*, MULTIPLY, INT_MAX, INT_MAX, int, true, 1); CHECK_SBINOP (*, MULTIPLY, INT_MAX, INT_MIN, int, true, INT_MIN); CHECK_SBINOP (*, MULTIPLY, INT_MIN, INT_MAX, int, true, INT_MIN); CHECK_SBINOP (*, MULTIPLY, INT_MIN, INT_MIN, int, true, 0); CHECK_SBINOP (*, MULTIPLY, -1, INT_MIN, int, INT_NEGATE_OVERFLOW (INT_MIN), INT_MIN); CHECK_SBINOP (*, MULTIPLY, LONG_MIN / INT_MAX, (long int) INT_MAX, long int, false, LONG_MIN - LONG_MIN % INT_MAX); CHECK_BINOP (/, DIVIDE, INT_MIN, -1, int, INT_NEGATE_OVERFLOW (INT_MIN), INT_MIN); CHECK_BINOP (/, DIVIDE, INT_MAX, 1, int, false, INT_MAX); CHECK_BINOP (/, DIVIDE, (unsigned int) INT_MIN, -1u, unsigned int, false, INT_MIN / -1u); CHECK_BINOP (%, REMAINDER, INT_MIN, -1, int, INT_NEGATE_OVERFLOW (INT_MIN), 0); CHECK_BINOP (%, REMAINDER, INT_MAX, 1, int, false, 0); CHECK_BINOP (%, REMAINDER, (unsigned int) INT_MIN, -1u, unsigned int, false, INT_MIN % -1u); CHECK_BINOP (<<, LEFT_SHIFT, UINT_MAX, 1, unsigned int, true, UINT_MAX << 1); CHECK_BINOP (<<, LEFT_SHIFT, UINT_MAX / 2 + 1, 1, unsigned int, true, (UINT_MAX / 2 + 1) << 1); CHECK_BINOP (<<, LEFT_SHIFT, UINT_MAX / 2, 1, unsigned int, false, (UINT_MAX / 2) << 1); /* INT__OVERFLOW and INT__WRAPV with mixed types. */ #define CHECK_SUM(a, b, t, v, vres) \ CHECK_SUM1(a, b, t, v, vres); \ CHECK_SUM1(b, a, t, v, vres) #define CHECK_SSUM(a, b, t, v, vres) \ CHECK_SSUM1(a, b, t, v, vres); \ CHECK_SSUM1(b, a, t, v, vres) #define CHECK_SUM1(a, b, t, v, vres) \ VERIFY (INT_ADD_OVERFLOW (a, b) == (v)) #define CHECK_SSUM1(a, b, t, v, vres) \ CHECK_SUM1(a, b, t, v, vres); \ { \ t result; \ ASSERT (INT_ADD_WRAPV (a, b, &result) == (v)); \ ASSERT (result == ((v) ? (vres) : ((a) + (b)))); \ } CHECK_SSUM (-1, LONG_MIN, long int, true, LONG_MAX); CHECK_SUM (-1, UINT_MAX, unsigned int, false, DONTCARE); CHECK_SSUM (-1L, INT_MIN, long int, INT_MIN == LONG_MIN, INT_MIN == LONG_MIN ? INT_MAX : DONTCARE); CHECK_SUM (0u, -1, unsigned int, true, 0u + -1); CHECK_SUM (0u, 0, unsigned int, false, DONTCARE); CHECK_SUM (0u, 1, unsigned int, false, DONTCARE); CHECK_SSUM (1, LONG_MAX, long int, true, LONG_MIN); CHECK_SUM (1, UINT_MAX, unsigned int, true, 0u); CHECK_SSUM (1L, INT_MAX, long int, INT_MAX == LONG_MAX, INT_MAX == LONG_MAX ? INT_MIN : DONTCARE); CHECK_SUM (1u, INT_MAX, unsigned int, INT_MAX == UINT_MAX, 1u + INT_MAX); CHECK_SUM (1u, INT_MIN, unsigned int, true, 1u + INT_MIN); { long int result; ASSERT (INT_ADD_WRAPV (1, INT_MAX, &result) == (INT_MAX == LONG_MAX)); ASSERT (INT_ADD_WRAPV (-1, INT_MIN, &result) == (INT_MIN == LONG_MIN)); } #define CHECK_DIFFERENCE(a, b, t, v, vres) \ VERIFY (INT_SUBTRACT_OVERFLOW (a, b) == (v)) #define CHECK_SDIFFERENCE(a, b, t, v, vres) \ CHECK_DIFFERENCE(a, b, t, v, vres); \ { \ t result; \ ASSERT (INT_SUBTRACT_WRAPV (a, b, &result) == (v)); \ ASSERT (result == ((v) ? (vres) : ((a) - (b)))); \ } CHECK_DIFFERENCE (INT_MAX, 1u, unsigned int, UINT_MAX < INT_MAX - 1, INT_MAX - 1u); CHECK_DIFFERENCE (UINT_MAX, 1, unsigned int, false, UINT_MAX - 1); CHECK_DIFFERENCE (0u, -1, unsigned int, false, 0u - -1); CHECK_DIFFERENCE (UINT_MAX, -1, unsigned int, true, UINT_MAX - -1); CHECK_DIFFERENCE (INT_MIN, 1u, unsigned int, true, INT_MIN - 1u); CHECK_DIFFERENCE (-1, 0u, unsigned int, true, -1 - 0u); CHECK_SDIFFERENCE (-1, INT_MIN, int, false, -1 - INT_MIN); CHECK_SDIFFERENCE (-1, INT_MAX, int, false, -1 - INT_MAX); CHECK_SDIFFERENCE (0, INT_MIN, int, INT_MIN < -INT_MAX, INT_MIN); CHECK_SDIFFERENCE (0, INT_MAX, int, false, 0 - INT_MAX); { long int result; ASSERT (INT_SUBTRACT_WRAPV (INT_MAX, -1, &result) == (INT_MAX == LONG_MAX)); ASSERT (INT_SUBTRACT_WRAPV (INT_MIN, 1, &result) == (INT_MAX == LONG_MAX)); } #define CHECK_PRODUCT(a, b, t, v, vres) \ CHECK_PRODUCT1(a, b, t, v, vres); \ CHECK_PRODUCT1(b, a, t, v, vres) #define CHECK_SPRODUCT(a, b, t, v, vres) \ CHECK_SPRODUCT1(a, b, t, v, vres); \ CHECK_SPRODUCT1(b, a, t, v, vres) #define CHECK_PRODUCT1(a, b, t, v, vres) \ VERIFY (INT_MULTIPLY_OVERFLOW (a, b) == (v)) #define CHECK_SPRODUCT1(a, b, t, v, vres) \ CHECK_PRODUCT1(a, b, t, v, vres); \ { \ t result; \ ASSERT (INT_MULTIPLY_WRAPV (a, b, &result) == (v)); \ ASSERT (result == ((v) ? (vres) : ((a) * (b)))); \ } CHECK_PRODUCT (-1, 1u, unsigned int, true, -1 * 1u); CHECK_SPRODUCT (-1, INT_MIN, int, INT_NEGATE_OVERFLOW (INT_MIN), INT_MIN); CHECK_PRODUCT (-1, UINT_MAX, unsigned int, true, -1 * UINT_MAX); CHECK_SPRODUCT (-32768, LONG_MAX / -32768 - 1, long int, true, LONG_MIN); CHECK_SPRODUCT (-12345, LONG_MAX / -12345, long int, false, DONTCARE); CHECK_SPRODUCT (0, -1, int, false, DONTCARE); CHECK_SPRODUCT (0, 0, int, false, DONTCARE); CHECK_PRODUCT (0, 0u, unsigned int, false, DONTCARE); CHECK_SPRODUCT (0, 1, int, false, DONTCARE); CHECK_SPRODUCT (0, INT_MAX, int, false, DONTCARE); CHECK_SPRODUCT (0, INT_MIN, int, false, DONTCARE); CHECK_PRODUCT (0, UINT_MAX, unsigned int, false, DONTCARE); CHECK_PRODUCT (0u, -1, unsigned int, false, DONTCARE); CHECK_PRODUCT (0u, 0, unsigned int, false, DONTCARE); CHECK_PRODUCT (0u, 0u, unsigned int, false, DONTCARE); CHECK_PRODUCT (0u, 1, unsigned int, false, DONTCARE); CHECK_PRODUCT (0u, INT_MAX, unsigned int, false, DONTCARE); CHECK_PRODUCT (0u, INT_MIN, unsigned int, false, DONTCARE); CHECK_PRODUCT (0u, UINT_MAX, unsigned int, false, DONTCARE); CHECK_SPRODUCT (1, INT_MAX, int, false, DONTCARE); CHECK_SPRODUCT (1, INT_MIN, int, false, DONTCARE); CHECK_PRODUCT (1, UINT_MAX, unsigned int, false, DONTCARE); CHECK_PRODUCT (1u, INT_MIN, unsigned int, true, 1u * INT_MIN); CHECK_PRODUCT (1u, INT_MAX, unsigned int, UINT_MAX < INT_MAX, 1u * INT_MAX); CHECK_PRODUCT (INT_MAX, UINT_MAX, unsigned int, true, INT_MAX * UINT_MAX); CHECK_PRODUCT (INT_MAX, ULONG_MAX, unsigned long int, true, INT_MAX * ULONG_MAX); CHECK_SPRODUCT (INT_MIN, LONG_MAX / INT_MIN - 1, long int, true, LONG_MIN); CHECK_SPRODUCT (INT_MIN, LONG_MAX / INT_MIN, long int, false, DONTCARE); CHECK_PRODUCT (INT_MIN, UINT_MAX, unsigned int, true, INT_MIN * UINT_MAX); CHECK_PRODUCT (INT_MIN, ULONG_MAX, unsigned long int, true, INT_MIN * ULONG_MAX); { long int result; ASSERT (INT_MULTIPLY_WRAPV (INT_MAX, INT_MAX, &result) == (LONG_MAX / INT_MAX < INT_MAX)); ASSERT (INT_MULTIPLY_WRAPV (INT_MAX, INT_MAX, &result) || result == INT_MAX * (long int) INT_MAX); ASSERT (INT_MULTIPLY_WRAPV (INT_MIN, INT_MIN, &result) || result == INT_MIN * (long int) INT_MIN); } # ifdef LLONG_MAX { long long int result; ASSERT (INT_MULTIPLY_WRAPV (LONG_MAX, LONG_MAX, &result) == (LLONG_MAX / LONG_MAX < LONG_MAX)); ASSERT (INT_MULTIPLY_WRAPV (LONG_MAX, LONG_MAX, &result) || result == LONG_MAX * (long long int) LONG_MAX); ASSERT (INT_MULTIPLY_WRAPV (LONG_MIN, LONG_MIN, &result) || result == LONG_MIN * (long long int) LONG_MIN); } # endif #define CHECK_QUOTIENT(a, b, v) VERIFY (INT_DIVIDE_OVERFLOW (a, b) == (v)) CHECK_QUOTIENT (INT_MIN, -1L, INT_MIN == LONG_MIN); CHECK_QUOTIENT (INT_MIN, UINT_MAX, false); CHECK_QUOTIENT (INTMAX_MIN, UINTMAX_MAX, false); CHECK_QUOTIENT (INTMAX_MIN, UINT_MAX, false); CHECK_QUOTIENT (-11, 10u, true); CHECK_QUOTIENT (-10, 10u, true); CHECK_QUOTIENT (-9, 10u, false); CHECK_QUOTIENT (11u, -10, true); CHECK_QUOTIENT (10u, -10, true); CHECK_QUOTIENT (9u, -10, false); #define CHECK_REMAINDER(a, b, v) VERIFY (INT_REMAINDER_OVERFLOW (a, b) == (v)) CHECK_REMAINDER (INT_MIN, -1L, INT_MIN == LONG_MIN); CHECK_REMAINDER (-1, UINT_MAX, true); CHECK_REMAINDER ((intmax_t) -1, UINTMAX_MAX, true); CHECK_REMAINDER (INTMAX_MIN, UINT_MAX, (INTMAX_MAX < UINT_MAX && - (unsigned int) INTMAX_MIN % UINT_MAX != 0)); CHECK_REMAINDER (INT_MIN, ULONG_MAX, INT_MIN % ULONG_MAX != 1); CHECK_REMAINDER (1u, -1, false); CHECK_REMAINDER (37*39u, -39, false); CHECK_REMAINDER (37*39u + 1, -39, true); CHECK_REMAINDER (37*39u - 1, -39, true); CHECK_REMAINDER (LONG_MAX, -INT_MAX, false); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-ignore-value.c0000644000175000017500000000365113004436755020517 00000000000000/* Test the "ignore-value" module. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake. */ #include #include "ignore-value.h" #include #ifndef _GL_ATTRIBUTE_RETURN_CHECK # if __GNUC__ < 3 || (__GNUC__ == 3 && __GNUC_MINOR__ < 4) # define _GL_ATTRIBUTE_RETURN_CHECK # else # define _GL_ATTRIBUTE_RETURN_CHECK __attribute__((__warn_unused_result__)) # endif #endif struct s { int i; }; static char doChar (void) _GL_ATTRIBUTE_RETURN_CHECK; static int doInt (void) _GL_ATTRIBUTE_RETURN_CHECK; static off_t doOff (void) _GL_ATTRIBUTE_RETURN_CHECK; static void *doPtr (void) _GL_ATTRIBUTE_RETURN_CHECK; static struct s doStruct (void) _GL_ATTRIBUTE_RETURN_CHECK; static char doChar (void) { return 0; } static int doInt (void) { return 0; } static off_t doOff (void) { return 0; } static void * doPtr (void) { return NULL; } static struct s doStruct (void) { static struct s s1; return s1; } int main (void) { /* If this test can compile with -Werror and the same warnings as the rest of the project, then we are properly silencing warnings about ignored return values. */ ignore_value (doChar ()); ignore_value (doInt ()); ignore_value (doOff ()); ignore_value (doPtr ()); ignore_value (doStruct ()); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-gettimeofday.c0000644000175000017500000000245013004436755020577 00000000000000/* * Copyright (C) 2005, 2007, 2009-2016 Free Software Foundation, Inc. * Written by Jim Meyering. * * This program is free software: you can redistribute it and/or modify * it under the terms of the GNU General Public License as published by * the Free Software Foundation; either version 3 of the License, or * (at your option) any later version. * * This program is distributed in the hope that it will be useful, * but WITHOUT ANY WARRANTY; without even the implied warranty of * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * GNU General Public License for more details. * * You should have received a copy of the GNU General Public License * along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (gettimeofday, int, (struct timeval *, GETTIMEOFDAY_TIMEZONE *)); #include #include #include int main (void) { time_t t = 0; struct tm *lt; struct tm saved_lt; struct timeval tv; lt = localtime (&t); saved_lt = *lt; gettimeofday (&tv, NULL); if (memcmp (lt, &saved_lt, sizeof (struct tm)) != 0) { fprintf (stderr, "gettimeofday still clobbers the localtime buffer!\n"); return 1; } return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-getprogname.c0000644000175000017500000000400113004436755020420 00000000000000/* Test the gnulib getprogname module. Copyright (C) 2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "getprogname.h" #include #include #ifdef __hpux # define STREQ(a, b) (strncmp (a, b, 14) == 0) #else # define STREQ(a, b) (strcmp (a, b) == 0) #endif int main (void) { char const *p = getprogname (); /* libtool creates a temporary executable whose name is sometimes prefixed with "lt-" (depends on the platform). But the name of the temporary executable is a detail that should not be visible to the end user and to the test suite. Remove this "lt-" prefix here. */ if (strncmp (p, "lt-", 3) == 0) p += 3; /* Note: You can make this test fail a) by running it on a case-insensitive file system (such as on Windows, Cygwin, or on Mac OS X with a case-insensitive HFS+ file system), with an invocation that contains upper case characters, e.g. test-GETPROGNAME, b) by hardlinking or symlinking it to a different name (e.g. test-foo) and invoking it through that name. That's not the intended use. The Makefile always invokes it as 'test-getprogname${EXEEXT}'. */ #if defined __CYGWIN__ /* The Cygwin getprogname() function strips the ".exe" suffix. */ assert (STREQ (p, "test-getprogname")); #else assert (STREQ (p, "test-getprogname" EXEEXT)); #endif return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-getopt.c0000644000175000017500000000547213004436755017427 00000000000000/* Test of command line argument processing. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ #include /* None of the files accessed by this test are large, so disable the ftell link warning if we are not using the gnulib ftell module. */ #define _GL_NO_LARGE_FILES #if GNULIB_TEST_GETOPT_GNU # include # ifndef __getopt_argv_const # define __getopt_argv_const const # endif # include "signature.h" SIGNATURE_CHECK (getopt_long, int, (int, char *__getopt_argv_const *, char const *, struct option const *, int *)); SIGNATURE_CHECK (getopt_long_only, int, (int, char *__getopt_argv_const *, char const *, struct option const *, int *)); #endif #include #include "signature.h" SIGNATURE_CHECK (getopt, int, (int, char * const[], char const *)); #include #include #include /* This test intentionally remaps stderr. So, we arrange to have fd 10 (outside the range of interesting fd's during the test) set up to duplicate the original stderr. */ #define BACKUP_STDERR_FILENO 10 #define ASSERT_STREAM myerr #include "macros.h" static FILE *myerr; #include "test-getopt.h" #if GNULIB_TEST_GETOPT_GNU # include "test-getopt_long.h" #endif int main (void) { /* This test validates that stderr is used correctly, so move the original into fd 10. */ if (dup2 (STDERR_FILENO, BACKUP_STDERR_FILENO) != BACKUP_STDERR_FILENO || (myerr = fdopen (BACKUP_STDERR_FILENO, "w")) == NULL) return 2; ASSERT (freopen ("test-getopt.tmp", "w", stderr) == stderr); /* These default values are required by POSIX. */ ASSERT (optind == 1); ASSERT (opterr != 0); setenv ("POSIXLY_CORRECT", "1", 1); test_getopt (); #if GNULIB_TEST_GETOPT_GNU test_getopt_long_posix (); #endif unsetenv ("POSIXLY_CORRECT"); test_getopt (); #if GNULIB_TEST_GETOPT_GNU test_getopt_long (); test_getopt_long_only (); #endif ASSERT (fclose (stderr) == 0); ASSERT (remove ("test-getopt.tmp") == 0); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-getdtablesize.c0000644000175000017500000000215013004436755020741 00000000000000/* Test of getdtablesize() function. Copyright (C) 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include #include "signature.h" SIGNATURE_CHECK (getdtablesize, int, (void)); #include "macros.h" int main (int argc, char *argv[]) { ASSERT (getdtablesize () >= 3); ASSERT (dup2 (0, getdtablesize() - 1) == getdtablesize () - 1); ASSERT (dup2 (0, getdtablesize()) == -1); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-getcwd-lgpl.c0000644000175000017500000000510513004436755020327 00000000000000/* Test of getcwd() function. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (getcwd, char *, (char *, size_t)); #include #include #include #include #include "macros.h" int main (int argc, char **argv) { char *pwd1; char *pwd2; /* If the user provides an argument, attempt to chdir there first. */ if (1 < argc) { if (chdir (argv[1]) == 0) printf ("changed to directory %s\n", argv[1]); } pwd1 = getcwd (NULL, 0); ASSERT (pwd1 && *pwd1); if (1 < argc) printf ("cwd=%s\n", pwd1); /* Make sure the result is usable. */ ASSERT (chdir (pwd1) == 0); ASSERT (chdir (".//./.") == 0); /* Make sure that result is normalized. */ pwd2 = getcwd (NULL, 0); ASSERT (pwd2); ASSERT (strcmp (pwd1, pwd2) == 0); free (pwd2); { size_t len = strlen (pwd1); ssize_t i = len - 10; if (i < 1) i = 1; pwd2 = getcwd (NULL, len + 1); ASSERT (pwd2); free (pwd2); pwd2 = malloc (len + 2); for ( ; i <= len; i++) { char *tmp; errno = 0; ASSERT (getcwd (pwd2, i) == NULL); ASSERT (errno == ERANGE); /* Allow either glibc or BSD behavior, since POSIX allows both. */ errno = 0; tmp = getcwd (NULL, i); if (tmp) { ASSERT (strcmp (pwd1, tmp) == 0); free (tmp); } else { ASSERT (errno == ERANGE); } } ASSERT (getcwd (pwd2, len + 1) == pwd2); pwd2[len] = '/'; pwd2[len + 1] = '\0'; } ASSERT (strstr (pwd2, "/./") == NULL); ASSERT (strstr (pwd2, "/../") == NULL); ASSERT (strstr (pwd2 + 1 + (pwd2[1] == '/'), "//") == NULL); /* Validate a POSIX requirement on size. */ errno = 0; ASSERT (getcwd(pwd2, 0) == NULL); ASSERT (errno == EINVAL); free (pwd1); free (pwd2); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-fwrite.c0000644000175000017500000000505013004436755017415 00000000000000/* Test of fwrite() function. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (fwrite, size_t, (const void *, size_t, size_t, FILE *)); #include #include #include #include "msvc-inval.h" #include "macros.h" int main (int argc, char **argv) { const char *filename = "test-fwrite.txt"; /* We don't have an fwrite() function that installs an invalid parameter handler so far. So install that handler here, explicitly. */ #if HAVE_MSVC_INVALID_PARAMETER_HANDLER \ && MSVC_INVALID_PARAMETER_HANDLING == DEFAULT_HANDLING gl_msvc_inval_ensure_handler (); #endif /* Test that fwrite() on an unbuffered stream sets errno if someone else closes the stream fd behind the back of stdio. */ { FILE *fp = fopen (filename, "w"); char buf[5] = "world"; ASSERT (fp != NULL); setvbuf (fp, NULL, _IONBF, 0); ASSERT (close (fileno (fp)) == 0); errno = 0; ASSERT (fwrite (buf, 1, sizeof (buf), fp) == 0); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } /* Test that fwrite() on an unbuffered stream sets errno if the stream was constructed with an invalid file descriptor. */ { FILE *fp = fdopen (-1, "w"); if (fp != NULL) { char buf[5] = "world"; setvbuf (fp, NULL, _IONBF, 0); errno = 0; ASSERT (fwrite (buf, 1, sizeof (buf), fp) == 0); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } { FILE *fp; close (99); fp = fdopen (99, "w"); if (fp != NULL) { char buf[5] = "world"; setvbuf (fp, NULL, _IONBF, 0); errno = 0; ASSERT (fwrite (buf, 1, sizeof (buf), fp) == 0); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } /* Clean up. */ unlink (filename); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-fstat.c0000644000175000017500000000237413004436755017244 00000000000000/* Tests of fstat() function. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (fstat, int, (int, struct stat *)); #include #include #include "macros.h" int main (int argc, char *argv[]) { /* Test behaviour for invalid file descriptors. */ { struct stat statbuf; errno = 0; ASSERT (fstat (-1, &statbuf) == -1); ASSERT (errno == EBADF); } { struct stat statbuf; close (99); errno = 0; ASSERT (fstat (99, &statbuf) == -1); ASSERT (errno == EBADF); } return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-fread.c0000644000175000017500000000510013004436755017172 00000000000000/* Test of fread() function. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (fread, size_t, (void *, size_t, size_t, FILE *)); #include #include #include #include "msvc-inval.h" #include "macros.h" int main (int argc, char **argv) { const char *filename = "test-fread.txt"; /* We don't have an fread() function that installs an invalid parameter handler so far. So install that handler here, explicitly. */ #if HAVE_MSVC_INVALID_PARAMETER_HANDLER \ && MSVC_INVALID_PARAMETER_HANDLING == DEFAULT_HANDLING gl_msvc_inval_ensure_handler (); #endif /* Prepare a file. */ { const char text[] = "hello world"; int fd = open (filename, O_RDWR | O_CREAT | O_TRUNC, 0600); ASSERT (fd >= 0); ASSERT (write (fd, text, sizeof (text)) == sizeof (text)); ASSERT (close (fd) == 0); } /* Test that fread() sets errno if someone else closes the stream fd behind the back of stdio. */ { FILE *fp = fopen (filename, "r"); char buf[5]; ASSERT (fp != NULL); ASSERT (close (fileno (fp)) == 0); errno = 0; ASSERT (fread (buf, 1, sizeof (buf), fp) == 0); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } /* Test that fread() sets errno if the stream was constructed with an invalid file descriptor. */ { FILE *fp = fdopen (-1, "r"); if (fp != NULL) { char buf[1]; errno = 0; ASSERT (fread (buf, 1, 1, fp) == 0); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } { FILE *fp; close (99); fp = fdopen (99, "r"); if (fp != NULL) { char buf[1]; errno = 0; ASSERT (fread (buf, 1, 1, fp) == 0); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } /* Clean up. */ unlink (filename); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-fputc.c0000644000175000017500000000457513004436755017251 00000000000000/* Test of fputc() function. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (fputc, int, (int, FILE *)); #include #include #include #include "msvc-inval.h" #include "macros.h" int main (int argc, char **argv) { const char *filename = "test-fputc.txt"; /* We don't have an fputc() function that installs an invalid parameter handler so far. So install that handler here, explicitly. */ #if HAVE_MSVC_INVALID_PARAMETER_HANDLER \ && MSVC_INVALID_PARAMETER_HANDLING == DEFAULT_HANDLING gl_msvc_inval_ensure_handler (); #endif /* Test that fputc() on an unbuffered stream sets errno if someone else closes the stream fd behind the back of stdio. */ { FILE *fp = fopen (filename, "w"); ASSERT (fp != NULL); setvbuf (fp, NULL, _IONBF, 0); ASSERT (close (fileno (fp)) == 0); errno = 0; ASSERT (fputc ('x', fp) == EOF); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } /* Test that fputc() on an unbuffered stream sets errno if the stream was constructed with an invalid file descriptor. */ { FILE *fp = fdopen (-1, "w"); if (fp != NULL) { setvbuf (fp, NULL, _IONBF, 0); errno = 0; ASSERT (fputc ('x', fp) == EOF); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } { FILE *fp; close (99); fp = fdopen (99, "w"); if (fp != NULL) { setvbuf (fp, NULL, _IONBF, 0); errno = 0; ASSERT (fputc ('x', fp) == EOF); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } /* Clean up. */ unlink (filename); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-float.c0000644000175000017500000002162413004436755017227 00000000000000/* Test of substitute. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2011. */ #include #include #include "fpucw.h" #include "macros.h" /* Check that FLT_RADIX is a constant expression. */ int a[] = { FLT_RADIX }; #if FLT_RADIX == 2 /* Return 2^n. */ static float pow2f (int n) { int k = n; volatile float x = 1; volatile float y = 2; /* Invariant: 2^n == x * y^k. */ if (k < 0) { y = 0.5f; k = - k; } while (k > 0) { if (k != 2 * (k / 2)) { x = x * y; k = k - 1; } if (k == 0) break; y = y * y; k = k / 2; } /* Now k == 0, hence x == 2^n. */ return x; } /* Return 2^n. */ static double pow2d (int n) { int k = n; volatile double x = 1; volatile double y = 2; /* Invariant: 2^n == x * y^k. */ if (k < 0) { y = 0.5; k = - k; } while (k > 0) { if (k != 2 * (k / 2)) { x = x * y; k = k - 1; } if (k == 0) break; y = y * y; k = k / 2; } /* Now k == 0, hence x == 2^n. */ return x; } /* Return 2^n. */ static long double pow2l (int n) { int k = n; volatile long double x = 1; volatile long double y = 2; /* Invariant: 2^n == x * y^k. */ if (k < 0) { y = 0.5L; k = - k; } while (k > 0) { if (k != 2 * (k / 2)) { x = x * y; k = k - 1; } if (k == 0) break; y = y * y; k = k / 2; } /* Now k == 0, hence x == 2^n. */ return x; } /* ----------------------- Check macros for 'float' ----------------------- */ /* Check that the FLT_* macros expand to constant expressions. */ int fb[] = { FLT_MANT_DIG, FLT_MIN_EXP, FLT_MAX_EXP, FLT_DIG, FLT_MIN_10_EXP, FLT_MAX_10_EXP }; float fc[] = { FLT_EPSILON, FLT_MIN, FLT_MAX }; static void test_float (void) { /* Check that the value of FLT_MIN_EXP is well parenthesized. */ ASSERT ((FLT_MIN_EXP % 101111) == (FLT_MIN_EXP) % 101111); /* Check that the value of DBL_MIN_10_EXP is well parenthesized. */ ASSERT ((FLT_MIN_10_EXP % 101111) == (FLT_MIN_10_EXP) % 101111); /* Check that 'float' is as specified in IEEE 754. */ ASSERT (FLT_MANT_DIG == 24); ASSERT (FLT_MIN_EXP == -125); ASSERT (FLT_MAX_EXP == 128); /* Check the value of FLT_MIN_10_EXP. */ ASSERT (FLT_MIN_10_EXP == - (int) (- (FLT_MIN_EXP - 1) * 0.30103)); /* Check the value of FLT_DIG. */ ASSERT (FLT_DIG == (int) ((FLT_MANT_DIG - 1) * 0.30103)); /* Check the value of FLT_MIN_10_EXP. */ ASSERT (FLT_MIN_10_EXP == - (int) (- (FLT_MIN_EXP - 1) * 0.30103)); /* Check the value of FLT_MAX_10_EXP. */ ASSERT (FLT_MAX_10_EXP == (int) (FLT_MAX_EXP * 0.30103)); /* Check the value of FLT_MAX. */ { volatile float m = FLT_MAX; int n; ASSERT (m + m > m); for (n = 0; n <= 2 * FLT_MANT_DIG; n++) { volatile float pow2_n = pow2f (n); /* 2^n */ volatile float x = m + (m / pow2_n); if (x > m) ASSERT (x + x == x); else ASSERT (!(x + x == x)); } } /* Check the value of FLT_MIN. */ { volatile float m = FLT_MIN; volatile float x = pow2f (FLT_MIN_EXP - 1); ASSERT (m == x); } /* Check the value of FLT_EPSILON. */ { volatile float e = FLT_EPSILON; volatile float me; int n; me = 1.0f + e; ASSERT (me > 1.0f); ASSERT (me - 1.0f == e); for (n = 0; n <= 2 * FLT_MANT_DIG; n++) { volatile float half_n = pow2f (- n); /* 2^-n */ volatile float x = me - half_n; if (x < me) ASSERT (x <= 1.0f); } } } /* ----------------------- Check macros for 'double' ----------------------- */ /* Check that the DBL_* macros expand to constant expressions. */ int db[] = { DBL_MANT_DIG, DBL_MIN_EXP, DBL_MAX_EXP, DBL_DIG, DBL_MIN_10_EXP, DBL_MAX_10_EXP }; double dc[] = { DBL_EPSILON, DBL_MIN, DBL_MAX }; static void test_double (void) { /* Check that the value of DBL_MIN_EXP is well parenthesized. */ ASSERT ((DBL_MIN_EXP % 101111) == (DBL_MIN_EXP) % 101111); /* Check that the value of DBL_MIN_10_EXP is well parenthesized. */ ASSERT ((DBL_MIN_10_EXP % 101111) == (DBL_MIN_10_EXP) % 101111); /* Check that 'double' is as specified in IEEE 754. */ ASSERT (DBL_MANT_DIG == 53); ASSERT (DBL_MIN_EXP == -1021); ASSERT (DBL_MAX_EXP == 1024); /* Check the value of DBL_MIN_10_EXP. */ ASSERT (DBL_MIN_10_EXP == - (int) (- (DBL_MIN_EXP - 1) * 0.30103)); /* Check the value of DBL_DIG. */ ASSERT (DBL_DIG == (int) ((DBL_MANT_DIG - 1) * 0.30103)); /* Check the value of DBL_MIN_10_EXP. */ ASSERT (DBL_MIN_10_EXP == - (int) (- (DBL_MIN_EXP - 1) * 0.30103)); /* Check the value of DBL_MAX_10_EXP. */ ASSERT (DBL_MAX_10_EXP == (int) (DBL_MAX_EXP * 0.30103)); /* Check the value of DBL_MAX. */ { volatile double m = DBL_MAX; int n; ASSERT (m + m > m); for (n = 0; n <= 2 * DBL_MANT_DIG; n++) { volatile double pow2_n = pow2d (n); /* 2^n */ volatile double x = m + (m / pow2_n); if (x > m) ASSERT (x + x == x); else ASSERT (!(x + x == x)); } } /* Check the value of DBL_MIN. */ { volatile double m = DBL_MIN; volatile double x = pow2d (DBL_MIN_EXP - 1); ASSERT (m == x); } /* Check the value of DBL_EPSILON. */ { volatile double e = DBL_EPSILON; volatile double me; int n; me = 1.0 + e; ASSERT (me > 1.0); ASSERT (me - 1.0 == e); for (n = 0; n <= 2 * DBL_MANT_DIG; n++) { volatile double half_n = pow2d (- n); /* 2^-n */ volatile double x = me - half_n; if (x < me) ASSERT (x <= 1.0); } } } /* -------------------- Check macros for 'long double' -------------------- */ /* Check that the LDBL_* macros expand to constant expressions. */ int lb[] = { LDBL_MANT_DIG, LDBL_MIN_EXP, LDBL_MAX_EXP, LDBL_DIG, LDBL_MIN_10_EXP, LDBL_MAX_10_EXP }; long double lc1 = LDBL_EPSILON; long double lc2 = LDBL_MIN; #if 0 /* LDBL_MAX is not a constant expression on some platforms. */ long double lc3 = LDBL_MAX; #endif static void test_long_double (void) { /* Check that the value of LDBL_MIN_EXP is well parenthesized. */ ASSERT ((LDBL_MIN_EXP % 101111) == (LDBL_MIN_EXP) % 101111); /* Check that the value of LDBL_MIN_10_EXP is well parenthesized. */ ASSERT ((LDBL_MIN_10_EXP % 101111) == (LDBL_MIN_10_EXP) % 101111); /* Check that 'long double' is at least as wide as 'double'. */ ASSERT (LDBL_MANT_DIG >= DBL_MANT_DIG); ASSERT (LDBL_MIN_EXP - LDBL_MANT_DIG <= DBL_MIN_EXP - DBL_MANT_DIG); ASSERT (LDBL_MAX_EXP >= DBL_MAX_EXP); /* Check the value of LDBL_DIG. */ ASSERT (LDBL_DIG == (int)((LDBL_MANT_DIG - 1) * 0.30103)); /* Check the value of LDBL_MIN_10_EXP. */ ASSERT (LDBL_MIN_10_EXP == - (int) (- (LDBL_MIN_EXP - 1) * 0.30103)); /* Check the value of LDBL_MAX_10_EXP. */ ASSERT (LDBL_MAX_10_EXP == (int) (LDBL_MAX_EXP * 0.30103)); /* Check the value of LDBL_MAX. */ { volatile long double m = LDBL_MAX; int n; ASSERT (m + m > m); for (n = 0; n <= 2 * LDBL_MANT_DIG; n++) { volatile long double pow2_n = pow2l (n); /* 2^n */ volatile long double x = m + (m / pow2_n); if (x > m) ASSERT (x + x == x); else ASSERT (!(x + x == x)); } } /* Check the value of LDBL_MIN. */ { volatile long double m = LDBL_MIN; volatile long double x = pow2l (LDBL_MIN_EXP - 1); ASSERT (m == x); } /* Check the value of LDBL_EPSILON. */ { volatile long double e = LDBL_EPSILON; volatile long double me; int n; me = 1.0L + e; ASSERT (me > 1.0L); ASSERT (me - 1.0L == e); for (n = 0; n <= 2 * LDBL_MANT_DIG; n++) { volatile long double half_n = pow2l (- n); /* 2^-n */ volatile long double x = me - half_n; if (x < me) ASSERT (x <= 1.0L); } } } int main () { test_float (); test_double (); { DECL_LONG_DOUBLE_ROUNDING BEGIN_LONG_DOUBLE_ROUNDING (); test_long_double (); END_LONG_DOUBLE_ROUNDING (); } return 0; } #else int main () { fprintf (stderr, "Skipping test: FLT_RADIX is not 2.\n"); return 77; } #endif gnuastro-0.2.33-8a3b/bootstrapped/tests/test-fgetc.c0000644000175000017500000000470413004436755017212 00000000000000/* Test of fgetc() function. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (fgetc, int, (FILE *)); #include #include #include #include "msvc-inval.h" #include "macros.h" int main (int argc, char **argv) { const char *filename = "test-fgetc.txt"; /* We don't have an fgetc() function that installs an invalid parameter handler so far. So install that handler here, explicitly. */ #if HAVE_MSVC_INVALID_PARAMETER_HANDLER \ && MSVC_INVALID_PARAMETER_HANDLING == DEFAULT_HANDLING gl_msvc_inval_ensure_handler (); #endif /* Prepare a file. */ { const char text[] = "hello world"; int fd = open (filename, O_RDWR | O_CREAT | O_TRUNC, 0600); ASSERT (fd >= 0); ASSERT (write (fd, text, sizeof (text)) == sizeof (text)); ASSERT (close (fd) == 0); } /* Test that fgetc() sets errno if someone else closes the stream fd behind the back of stdio. */ { FILE *fp = fopen (filename, "r"); ASSERT (fp != NULL); ASSERT (close (fileno (fp)) == 0); errno = 0; ASSERT (fgetc (fp) == EOF); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } /* Test that fgetc() sets errno if the stream was constructed with an invalid file descriptor. */ { FILE *fp = fdopen (-1, "r"); if (fp != NULL) { errno = 0; ASSERT (fgetc (fp) == EOF); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } { FILE *fp; close (99); fp = fdopen (99, "r"); if (fp != NULL) { errno = 0; ASSERT (fgetc (fp) == EOF); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } /* Clean up. */ unlink (filename); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-fdopen.c0000644000175000017500000000255613004436755017400 00000000000000/* Test opening a stream with a file descriptor. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (fdopen, FILE *, (int, const char *)); #include #include #include "macros.h" int main (void) { /* Test behavior on failure. POSIX makes it hard to check for failure, since the behavior is not well-defined on invalid file descriptors, so try fdopen 1000 times and if that's not enough to fail due to EMFILE, so be it. */ int i; for (i = 0; i < 1000; i++) { errno = 0; if (! fdopen (STDOUT_FILENO, "w")) { ASSERT (errno != 0); break; } } return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-fcntl-h.c0000644000175000017500000000552413004436755017456 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include /* Check that the various O_* macros are defined. */ int o = (O_DIRECT | O_DIRECTORY | O_DSYNC | O_IGNORE_CTTY | O_NDELAY | O_NOATIME | O_NONBLOCK | O_NOCTTY | O_NOFOLLOW | O_NOLINK | O_NOLINKS | O_NOTRANS | O_RSYNC | O_SYNC | O_TTY_INIT | O_BINARY | O_TEXT); /* Check that the various SEEK_* macros are defined. */ int sk[] = { SEEK_CUR, SEEK_END, SEEK_SET }; /* Check that the FD_* macros are defined. */ int i = FD_CLOEXEC; /* Check that the types are all defined. */ pid_t t1; off_t t2; mode_t t3; int main (void) { /* Ensure no overlap in SEEK_*. */ switch (0) { case SEEK_CUR: case SEEK_END: case SEEK_SET: ; } /* Ensure no dangerous overlap in non-zero gnulib-defined replacements. */ switch (O_RDONLY) { /* Access modes */ case O_RDONLY: case O_WRONLY: case O_RDWR: #if O_EXEC && O_EXEC != O_RDONLY case O_EXEC: #endif #if O_SEARCH && O_EXEC != O_SEARCH && O_SEARCH != O_RDONLY case O_SEARCH: #endif i = ! (~O_ACCMODE & (O_RDONLY | O_WRONLY | O_RDWR | O_EXEC | O_SEARCH)); break; /* Everyone should have these */ case O_CREAT: case O_EXCL: case O_TRUNC: case O_APPEND: break; /* These might be 0 or O_RDONLY, only test non-zero versions. */ #if O_CLOEXEC case O_CLOEXEC: #endif #if O_DIRECT case O_DIRECT: #endif #if O_DIRECTORY case O_DIRECTORY: #endif #if O_DSYNC case O_DSYNC: #endif #if O_IGNORE_CTTY case O_IGNORE_CTTY: #endif #if O_NOATIME case O_NOATIME: #endif #if O_NONBLOCK case O_NONBLOCK: #endif #if O_NOCTTY case O_NOCTTY: #endif #if O_NOFOLLOW case O_NOFOLLOW: #endif #if O_NOLINK case O_NOLINK: #endif #if O_NOLINKS case O_NOLINKS: #endif #if O_NOTRANS case O_NOTRANS: #endif #if O_RSYNC && O_RSYNC != O_DSYNC case O_RSYNC: #endif #if O_SYNC && O_SYNC != O_DSYNC && O_SYNC != O_RSYNC case O_SYNC: #endif #if O_TTY_INIT case O_TTY_INIT: #endif #if O_BINARY case O_BINARY: #endif #if O_TEXT case O_TEXT: #endif ; } return !i; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-errno.c0000644000175000017500000000555413004436755017253 00000000000000/* Test of substitute. Copyright (C) 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include /* Verify that the POSIX mandated errno values exist and can be used as initializers outside of a function. The variable names happen to match the Linux/x86 error numbers. */ int e1 = EPERM; int e2 = ENOENT; int e3 = ESRCH; int e4 = EINTR; int e5 = EIO; int e6 = ENXIO; int e7 = E2BIG; int e8 = ENOEXEC; int e9 = EBADF; int e10 = ECHILD; int e11 = EAGAIN; int e11a = EWOULDBLOCK; int e12 = ENOMEM; int e13 = EACCES; int e14 = EFAULT; int e16 = EBUSY; int e17 = EEXIST; int e18 = EXDEV; int e19 = ENODEV; int e20 = ENOTDIR; int e21 = EISDIR; int e22 = EINVAL; int e23 = ENFILE; int e24 = EMFILE; int e25 = ENOTTY; int e26 = ETXTBSY; int e27 = EFBIG; int e28 = ENOSPC; int e29 = ESPIPE; int e30 = EROFS; int e31 = EMLINK; int e32 = EPIPE; int e33 = EDOM; int e34 = ERANGE; int e35 = EDEADLK; int e36 = ENAMETOOLONG; int e37 = ENOLCK; int e38 = ENOSYS; int e39 = ENOTEMPTY; int e40 = ELOOP; int e42 = ENOMSG; int e43 = EIDRM; int e67 = ENOLINK; int e71 = EPROTO; int e72 = EMULTIHOP; int e74 = EBADMSG; int e75 = EOVERFLOW; int e84 = EILSEQ; int e88 = ENOTSOCK; int e89 = EDESTADDRREQ; int e90 = EMSGSIZE; int e91 = EPROTOTYPE; int e92 = ENOPROTOOPT; int e93 = EPROTONOSUPPORT; int e95 = EOPNOTSUPP; int e95a = ENOTSUP; int e97 = EAFNOSUPPORT; int e98 = EADDRINUSE; int e99 = EADDRNOTAVAIL; int e100 = ENETDOWN; int e101 = ENETUNREACH; int e102 = ENETRESET; int e103 = ECONNABORTED; int e104 = ECONNRESET; int e105 = ENOBUFS; int e106 = EISCONN; int e107 = ENOTCONN; int e110 = ETIMEDOUT; int e111 = ECONNREFUSED; int e113 = EHOSTUNREACH; int e114 = EALREADY; int e115 = EINPROGRESS; int e116 = ESTALE; int e122 = EDQUOT; int e125 = ECANCELED; int e130 = EOWNERDEAD; int e131 = ENOTRECOVERABLE; /* Don't verify that these errno values are all different, except for possibly EWOULDBLOCK == EAGAIN. Even Linux/x86 does not pass this check: it has ENOTSUP == EOPNOTSUPP. */ int main () { /* Verify that errno can be assigned. */ errno = EOVERFLOW; /* snprintf() callers want to distinguish EINVAL and EOVERFLOW. */ if (errno == EINVAL) return 1; return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-environ.c0000644000175000017500000000272713004436755017605 00000000000000/* Test of environ variable. Copyright (C) 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include #include int main () { /* The environment variables that are set even in the weirdest situations are HOME and PATH. POSIX says that HOME is initialized by the system, and that PATH may be unset. But in practice it's more frequent to see HOME unset and PATH set. So we test the presence of PATH. */ char **remaining_variables = environ; char *string; for (; (string = *remaining_variables) != NULL; remaining_variables++) { if (strncmp (string, "PATH=", 5) == 0) /* Found the PATH environment variable. */ return 0; } /* Failed to find the PATH environment variable. */ return 1; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-dup2.c0000644000175000017500000001376613004436755017004 00000000000000/* Test duplicating file descriptors. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include #include "signature.h" SIGNATURE_CHECK (dup2, int, (int, int)); #include #include #if HAVE_SYS_RESOURCE_H # include #endif #include "binary-io.h" #if GNULIB_TEST_CLOEXEC # include "cloexec.h" #endif #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Get declarations of the native Windows API functions. */ # define WIN32_LEAN_AND_MEAN # include /* Get _get_osfhandle. */ # include "msvc-nothrow.h" #endif #include "macros.h" /* Return non-zero if FD is open. */ static int is_open (int fd) { #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* On native Windows, the initial state of unassigned standard file descriptors is that they are open but point to an INVALID_HANDLE_VALUE, and there is no fcntl. */ return (HANDLE) _get_osfhandle (fd) != INVALID_HANDLE_VALUE; #else # ifndef F_GETFL # error Please port fcntl to your platform # endif return 0 <= fcntl (fd, F_GETFL); #endif } #if GNULIB_TEST_CLOEXEC /* Return non-zero if FD is open and inheritable across exec/spawn. */ static int is_inheritable (int fd) { # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* On native Windows, the initial state of unassigned standard file descriptors is that they are open but point to an INVALID_HANDLE_VALUE, and there is no fcntl. */ HANDLE h = (HANDLE) _get_osfhandle (fd); DWORD flags; if (h == INVALID_HANDLE_VALUE || GetHandleInformation (h, &flags) == 0) return 0; return (flags & HANDLE_FLAG_INHERIT) != 0; # else # ifndef F_GETFD # error Please port fcntl to your platform # endif int i = fcntl (fd, F_GETFD); return 0 <= i && (i & FD_CLOEXEC) == 0; # endif } #endif /* GNULIB_TEST_CLOEXEC */ #if !O_BINARY # define setmode(f,m) zero () static int zero (void) { return 0; } #endif /* Return non-zero if FD is open in the given MODE, which is either O_TEXT or O_BINARY. */ static int is_mode (int fd, int mode) { int value = setmode (fd, O_BINARY); setmode (fd, value); return mode == value; } int main (void) { const char *file = "test-dup2.tmp"; char buffer[1]; int bad_fd = getdtablesize (); int fd = open (file, O_CREAT | O_TRUNC | O_RDWR, 0600); /* Assume std descriptors were provided by invoker. */ ASSERT (STDERR_FILENO < fd); ASSERT (is_open (fd)); /* Ignore any other fd's leaked into this process. */ close (fd + 1); close (fd + 2); ASSERT (!is_open (fd + 1)); ASSERT (!is_open (fd + 2)); /* Assigning to self must be a no-op. */ ASSERT (dup2 (fd, fd) == fd); ASSERT (is_open (fd)); /* The source must be valid. */ errno = 0; ASSERT (dup2 (-1, fd) == -1); ASSERT (errno == EBADF); close (99); errno = 0; ASSERT (dup2 (99, fd) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (dup2 (AT_FDCWD, fd) == -1); ASSERT (errno == EBADF); ASSERT (is_open (fd)); /* If the source is not open, then the destination is unaffected. */ errno = 0; ASSERT (dup2 (fd + 1, fd + 1) == -1); ASSERT (errno == EBADF); ASSERT (!is_open (fd + 1)); errno = 0; ASSERT (dup2 (fd + 1, fd) == -1); ASSERT (errno == EBADF); ASSERT (is_open (fd)); /* The destination must be valid. */ errno = 0; ASSERT (dup2 (fd, -2) == -1); ASSERT (errno == EBADF); if (bad_fd > 256) { ASSERT (dup2 (fd, 255) == 255); ASSERT (dup2 (fd, 256) == 256); ASSERT (close (255) == 0); ASSERT (close (256) == 0); } ASSERT (dup2 (fd, bad_fd - 1) == bad_fd - 1); ASSERT (close (bad_fd - 1) == 0); errno = 0; ASSERT (dup2 (fd, bad_fd) == -1); ASSERT (errno == EBADF); /* Using dup2 can skip fds. */ ASSERT (dup2 (fd, fd + 2) == fd + 2); ASSERT (is_open (fd)); ASSERT (!is_open (fd + 1)); ASSERT (is_open (fd + 2)); /* Verify that dup2 closes the previous occupant of a fd. */ ASSERT (open ("/dev/null", O_WRONLY, 0600) == fd + 1); ASSERT (dup2 (fd + 1, fd) == fd); ASSERT (close (fd + 1) == 0); ASSERT (write (fd, "1", 1) == 1); ASSERT (dup2 (fd + 2, fd) == fd); ASSERT (lseek (fd, 0, SEEK_END) == 0); ASSERT (write (fd + 2, "2", 1) == 1); ASSERT (lseek (fd, 0, SEEK_SET) == 0); ASSERT (read (fd, buffer, 1) == 1); ASSERT (*buffer == '2'); #if GNULIB_TEST_CLOEXEC /* Any new fd created by dup2 must not be cloexec. */ ASSERT (close (fd + 2) == 0); ASSERT (dup_cloexec (fd) == fd + 1); ASSERT (!is_inheritable (fd + 1)); ASSERT (dup2 (fd + 1, fd + 1) == fd + 1); ASSERT (!is_inheritable (fd + 1)); ASSERT (dup2 (fd + 1, fd + 2) == fd + 2); ASSERT (!is_inheritable (fd + 1)); ASSERT (is_inheritable (fd + 2)); errno = 0; ASSERT (dup2 (fd + 1, -1) == -1); ASSERT (errno == EBADF); ASSERT (!is_inheritable (fd + 1)); #endif /* On systems that distinguish between text and binary mode, dup2 reuses the mode of the source. */ setmode (fd, O_BINARY); ASSERT (is_mode (fd, O_BINARY)); ASSERT (dup2 (fd, fd + 1) == fd + 1); ASSERT (is_mode (fd + 1, O_BINARY)); setmode (fd, O_TEXT); ASSERT (is_mode (fd, O_TEXT)); ASSERT (dup2 (fd, fd + 1) == fd + 1); ASSERT (is_mode (fd + 1, O_TEXT)); /* Clean up. */ ASSERT (close (fd + 2) == 0); ASSERT (close (fd + 1) == 0); ASSERT (close (fd) == 0); ASSERT (unlink (file) == 0); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-ctype.c0000644000175000017500000000154013004436755017241 00000000000000/* Test of substitute. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include int main (void) { return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-close.c0000644000175000017500000000220113004436755017215 00000000000000/* Test closing a file or socket. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (close, int, (int)); #include #include "macros.h" int main (void) { /* Test behaviour for invalid file descriptors. */ { errno = 0; ASSERT (close (-1) == -1); ASSERT (errno == EBADF); } { close (99); errno = 0; ASSERT (close (99) == -1); ASSERT (errno == EBADF); } return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-c-strncasecmp.c0000644000175000017500000000601013004436755020654 00000000000000/* Test of case-insensitive string comparison function. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include "c-strcase.h" #include "c-ctype.h" #include #include #include "macros.h" int main (int argc, char *argv[]) { if (argc > 1) { /* configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; } ASSERT (c_strncasecmp ("paragraph", "Paragraph", 1000000) == 0); ASSERT (c_strncasecmp ("paragraph", "Paragraph", 9) == 0); ASSERT (c_strncasecmp ("paragrapH", "parAgRaph", 1000000) == 0); ASSERT (c_strncasecmp ("paragrapH", "parAgRaph", 9) == 0); ASSERT (c_strncasecmp ("paragraph", "paraLyzed", 10) < 0); ASSERT (c_strncasecmp ("paragraph", "paraLyzed", 9) < 0); ASSERT (c_strncasecmp ("paragraph", "paraLyzed", 5) < 0); ASSERT (c_strncasecmp ("paragraph", "paraLyzed", 4) == 0); ASSERT (c_strncasecmp ("paraLyzed", "paragraph", 10) > 0); ASSERT (c_strncasecmp ("paraLyzed", "paragraph", 9) > 0); ASSERT (c_strncasecmp ("paraLyzed", "paragraph", 5) > 0); ASSERT (c_strncasecmp ("paraLyzed", "paragraph", 4) == 0); ASSERT (c_strncasecmp ("para", "paragraph", 10) < 0); ASSERT (c_strncasecmp ("para", "paragraph", 9) < 0); ASSERT (c_strncasecmp ("para", "paragraph", 5) < 0); ASSERT (c_strncasecmp ("para", "paragraph", 4) == 0); ASSERT (c_strncasecmp ("paragraph", "para", 10) > 0); ASSERT (c_strncasecmp ("paragraph", "para", 9) > 0); ASSERT (c_strncasecmp ("paragraph", "para", 5) > 0); ASSERT (c_strncasecmp ("paragraph", "para", 4) == 0); /* The following tests shows how c_strncasecmp() is different from strncasecmp(). */ ASSERT (c_strncasecmp ("\311mily", "\351mile", 4) < 0); ASSERT (c_strncasecmp ("\351mile", "\311mily", 4) > 0); /* The following tests shows how c_strncasecmp() is different from mbsncasecmp(). */ ASSERT (c_strncasecmp ("\303\266zg\303\274r", "\303\226ZG\303\234R", 99) > 0); /* özgür */ ASSERT (c_strncasecmp ("\303\226ZG\303\234R", "\303\266zg\303\274r", 99) < 0); /* özgür */ #if C_CTYPE_ASCII /* This test shows how strings of different size cannot compare equal. */ ASSERT (c_strncasecmp ("turkish", "TURK\304\260SH", 7) < 0); ASSERT (c_strncasecmp ("TURK\304\260SH", "turkish", 7) > 0); #endif return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-c-strcasecmp.c0000644000175000017500000000422213004436755020501 00000000000000/* Test of case-insensitive string comparison function. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include "c-strcase.h" #include "c-ctype.h" #include #include #include "macros.h" int main (int argc, char *argv[]) { if (argc > 1) { /* configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; } ASSERT (c_strcasecmp ("paragraph", "Paragraph") == 0); ASSERT (c_strcasecmp ("paragrapH", "parAgRaph") == 0); ASSERT (c_strcasecmp ("paragraph", "paraLyzed") < 0); ASSERT (c_strcasecmp ("paraLyzed", "paragraph") > 0); ASSERT (c_strcasecmp ("para", "paragraph") < 0); ASSERT (c_strcasecmp ("paragraph", "para") > 0); /* The following tests shows how c_strcasecmp() is different from strcasecmp(). */ ASSERT (c_strcasecmp ("\311mile", "\351mile") < 0); ASSERT (c_strcasecmp ("\351mile", "\311mile") > 0); /* The following tests shows how c_strcasecmp() is different from mbscasecmp(). */ ASSERT (c_strcasecmp ("\303\266zg\303\274r", "\303\226ZG\303\234R") > 0); /* özgür */ ASSERT (c_strcasecmp ("\303\226ZG\303\234R", "\303\266zg\303\274r") < 0); /* özgür */ #if C_CTYPE_ASCII /* This test shows how strings of different size cannot compare equal. */ ASSERT (c_strcasecmp ("turkish", "TURK\304\260SH") < 0); ASSERT (c_strcasecmp ("TURK\304\260SH", "turkish") > 0); #endif return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-c-ctype.c0000644000175000017500000001464313004436755017471 00000000000000/* Test of character handling in C locale. Copyright (C) 2005, 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2005. */ #include #include "c-ctype.h" #include #include #include #include "macros.h" static void test_agree_with_C_locale (void) { int c; for (c = 0; c <= UCHAR_MAX; c++) { ASSERT (c_isascii (c) == (isascii (c) != 0)); if (c_isascii (c)) { ASSERT (c_isalnum (c) == (isalnum (c) != 0)); ASSERT (c_isalpha (c) == (isalpha (c) != 0)); ASSERT (c_isblank (c) == (isblank (c) != 0)); ASSERT (c_iscntrl (c) == (iscntrl (c) != 0)); ASSERT (c_isdigit (c) == (isdigit (c) != 0)); ASSERT (c_islower (c) == (islower (c) != 0)); ASSERT (c_isgraph (c) == (isgraph (c) != 0)); ASSERT (c_isprint (c) == (isprint (c) != 0)); ASSERT (c_ispunct (c) == (ispunct (c) != 0)); ASSERT (c_isspace (c) == (isspace (c) != 0)); ASSERT (c_isupper (c) == (isupper (c) != 0)); ASSERT (c_isxdigit (c) == (isxdigit (c) != 0)); ASSERT (c_tolower (c) == tolower (c)); ASSERT (c_toupper (c) == toupper (c)); } } } static void test_all (void) { int c; int n_isascii = 0; for (c = CHAR_MIN; c <= UCHAR_MAX; c++) { if (! (0 <= c && c <= CHAR_MAX)) { ASSERT (! c_isascii (c)); ASSERT (! c_isalnum (c)); ASSERT (! c_isalpha (c)); ASSERT (! c_isblank (c)); ASSERT (! c_iscntrl (c)); ASSERT (! c_isdigit (c)); ASSERT (! c_islower (c)); ASSERT (! c_isgraph (c)); ASSERT (! c_isprint (c)); ASSERT (! c_ispunct (c)); ASSERT (! c_isspace (c)); ASSERT (! c_isupper (c)); ASSERT (! c_isxdigit (c)); ASSERT (c_tolower (c) == c); ASSERT (c_toupper (c) == c); } n_isascii += c_isascii (c); #ifdef C_CTYPE_ASCII ASSERT (c_isascii (c) == (0 <= c && c <= 0x7f)); #endif ASSERT (c_isascii (c) == (c_isprint (c) || c_iscntrl (c))); ASSERT (c_isalnum (c) == (c_isalpha (c) || c_isdigit (c))); ASSERT (c_isalpha (c) == (c_islower (c) || c_isupper (c))); switch (c) { case '\t': case ' ': ASSERT (c_isblank (c) == 1); break; default: ASSERT (c_isblank (c) == 0); break; } #ifdef C_CTYPE_ASCII ASSERT (c_iscntrl (c) == ((c >= 0 && c < 0x20) || c == 0x7f)); #endif switch (c) { case '\a': case '\b': case '\f': case '\n': case '\r': case '\t': case '\v': ASSERT (c_iscntrl (c)); break; } ASSERT (! (c_iscntrl (c) && c_isprint (c))); switch (c) { case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': ASSERT (c_isdigit (c) == 1); break; default: ASSERT (c_isdigit (c) == 0); break; } switch (c) { case 'a': case 'b': case 'c': case 'd': case 'e': case 'f': case 'g': case 'h': case 'i': case 'j': case 'k': case 'l': case 'm': case 'n': case 'o': case 'p': case 'q': case 'r': case 's': case 't': case 'u': case 'v': case 'w': case 'x': case 'y': case 'z': ASSERT (c_islower (c) == 1); ASSERT (c_toupper (c) == c - 'a' + 'A'); break; default: ASSERT (c_islower (c) == 0); ASSERT (c_toupper (c) == c); break; } #ifdef C_CTYPE_ASCII ASSERT (c_isgraph (c) == ((c >= 0x20 && c < 0x7f) && c != ' ')); ASSERT (c_isprint (c) == (c >= 0x20 && c < 0x7f)); #endif ASSERT (c_isgraph (c) == (c_isalnum (c) || c_ispunct (c))); ASSERT (c_isprint (c) == (c_isgraph (c) || c == ' ')); switch (c) { case '!': case '"': case '#': case '$': case '%': case '&': case '\'': case '(': case ')': case '*': case '+': case ',': case '-': case '.': case '/': case ':': case ';': case '<': case '=': case '>': case '?': case '@': case '[': case'\\': case ']': case '^': case '_': case '`': case '{': case '|': case '}': case '~': ASSERT (c_ispunct (c) == 1); break; default: ASSERT (c_ispunct (c) == 0); break; } switch (c) { case ' ': case '\t': case '\n': case '\v': case '\f': case '\r': ASSERT (c_isspace (c) == 1); break; default: ASSERT (c_isspace (c) == 0); break; } switch (c) { case 'A': case 'B': case 'C': case 'D': case 'E': case 'F': case 'G': case 'H': case 'I': case 'J': case 'K': case 'L': case 'M': case 'N': case 'O': case 'P': case 'Q': case 'R': case 'S': case 'T': case 'U': case 'V': case 'W': case 'X': case 'Y': case 'Z': ASSERT (c_isupper (c) == 1); ASSERT (c_tolower (c) == c - 'A' + 'a'); break; default: ASSERT (c_isupper (c) == 0); ASSERT (c_tolower (c) == c); break; } switch (c) { case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': case 'A': case 'B': case 'C': case 'D': case 'E': case 'F': case 'a': case 'b': case 'c': case 'd': case 'e': case 'f': ASSERT (c_isxdigit (c) == 1); break; default: ASSERT (c_isxdigit (c) == 0); break; } } ASSERT (n_isascii == 128); } int main () { test_agree_with_C_locale (); test_all (); setlocale (LC_ALL, "de_DE"); test_all (); setlocale (LC_ALL, "ja_JP.EUC-JP"); test_all (); return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-btowc.c0000644000175000017500000000331013004436755017230 00000000000000/* Test of conversion of unibyte character to wide character. Copyright (C) 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include #include "signature.h" SIGNATURE_CHECK (btowc, wint_t, (int)); #include #include #include "macros.h" int main (int argc, char *argv[]) { int c; /* configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; ASSERT (btowc (EOF) == WEOF); if (argc > 1) switch (argv[1][0]) { case '1': /* Locale encoding is ISO-8859-1 or ISO-8859-15. */ for (c = 0; c < 0x80; c++) ASSERT (btowc (c) == c); for (c = 0xA0; c < 0x100; c++) ASSERT (btowc (c) != WEOF); return 0; case '2': /* Locale encoding is UTF-8. */ for (c = 0; c < 0x80; c++) ASSERT (btowc (c) == c); for (c = 0x80; c < 0x100; c++) ASSERT (btowc (c) == WEOF); return 0; } return 1; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-binary-io.c0000644000175000017500000000324613004436755020013 00000000000000/* Test of binary mode I/O. Copyright (C) 2005, 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2005. */ #include #include "binary-io.h" #include #include #include #include #include #include #include "macros.h" int main (int argc, char *argv[]) { /* Test the O_BINARY macro. */ { int fd = open ("t-bin-out0.tmp", O_CREAT | O_TRUNC | O_RDWR | O_BINARY, 0600); if (write (fd, "Hello\n", 6) < 0) exit (1); close (fd); } { struct stat statbuf; if (stat ("t-bin-out0.tmp", &statbuf) < 0) exit (1); ASSERT (statbuf.st_size == 6); } switch (argv[1][0]) { case '1': /* Test the set_binary_mode() function. */ set_binary_mode (1, O_BINARY); fputs ("Hello\n", stdout); break; case '2': /* Test the SET_BINARY macro. */ SET_BINARY (1); fputs ("Hello\n", stdout); break; default: break; } return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-argp.c0000644000175000017500000002425413004436755017055 00000000000000/* Test suite for argp. Copyright (C) 2006-2007, 2009-2016 Free Software Foundation, Inc. This file is part of the GNUlib Library. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "argp.h" #include #include #include #if HAVE_STRINGS_H # include #endif struct test_args { int test; int verbose; char *file; int read; char *hidden; int opt; char *optional; int optional_set; int group_2_1_option; int group_1_1_option; }; static struct argp_option group1_option[] = { { NULL, 0, NULL, 0, "Option Group 1", 0 }, { "verbose", 'v', NULL, 0, "Simple option without arguments", 1 }, { "file", 'f', "FILE", 0, "Option with a mandatory argument", 1 }, { "input", 0, NULL, OPTION_ALIAS, NULL, 1 }, { "read", 'r', NULL, OPTION_ALIAS, NULL, 1 }, { "hidden", 'H', "FILE", OPTION_HIDDEN, "Hidden option", 1 }, { NULL, 0, NULL, 0, NULL, 0 } }; static error_t group1_parser (int key, char *arg, struct argp_state *state) { struct test_args *args = state->input; switch (key) { case 'v': args->verbose++; break; case 'r': args->read = 1; /* fall through */ case 'f': args->file = arg; break; case 'H': args->hidden = arg; break; default: return ARGP_ERR_UNKNOWN; } return 0; } struct argp group1_argp = { group1_option, group1_parser }; struct argp_child group1_child = { &group1_argp, 0, "", 1 }; static struct argp_option group1_1_option[] = { { NULL, 0, NULL, 0, "Option Group 1.1", 0 }, { "cantiga", 'C', NULL, 0, "create a cantiga" }, { "sonet", 'S', NULL, 0, "create a sonet" }, { NULL, 0, NULL, 0, NULL, 0 } }; static error_t group1_1_parser (int key, char *arg, struct argp_state *state) { struct test_args *args = state->input; switch (key) { case 'C': case 'S': args->group_1_1_option = key; break; default: return ARGP_ERR_UNKNOWN; } return 0; } struct argp group1_1_argp = { group1_1_option, group1_1_parser }; struct argp_child group1_1_child = { &group1_1_argp, 0, "", 2 }; static struct argp_option group2_option[] = { { NULL, 0, NULL, 0, "Option Group 2", 0 }, { "option", 'O', NULL, 0, "An option", 1 }, { "optional", 'o', "ARG", OPTION_ARG_OPTIONAL, "Option with an optional argument. ARG is one of the following:", 2 }, { "one", 0, NULL, OPTION_DOC | OPTION_NO_TRANS, "one unit", 3 }, { "two", 0, NULL, OPTION_DOC | OPTION_NO_TRANS, "two units", 3 }, { "many", 0, NULL, OPTION_DOC | OPTION_NO_TRANS, "many units", 3 }, { NULL, 0, NULL, 0, NULL, 0 } }; static error_t group2_parser (int key, char *arg, struct argp_state *state) { struct test_args *args = state->input; switch (key) { case 'O': args->opt = 1; break; case 'o': args->optional_set = 1; args->optional = arg; break; default: return ARGP_ERR_UNKNOWN; } return 0; } struct argp group2_argp = { group2_option, group2_parser }; struct argp_child group2_child = { &group2_argp, 0, "", 2 }; static struct argp_option group2_1_option[] = { { NULL, 0, NULL, 0, "Option Group 2.1", 0 }, { "poem", 'p', NULL, 0, "create a poem" }, { "limerick", 'l', NULL, 0, "create a limerick" }, { NULL, 0, NULL, 0, NULL, 0 } }; static error_t group2_1_parser (int key, char *arg, struct argp_state *state) { struct test_args *args = state->input; switch (key) { case 'p': case 'e': args->group_2_1_option = key; break; default: return ARGP_ERR_UNKNOWN; } return 0; } struct argp group2_1_argp = { group2_1_option, group2_1_parser }; struct argp_child group2_1_child = { &group2_1_argp, 0, "", 2 }; static struct argp_option main_options[] = { { NULL, 0, NULL, 0, "Main options", 0 }, { "test", 't', NULL, 0, NULL, 1 }, { NULL, 0, NULL, 0, NULL, 0 } }; static error_t parse_opt (int key, char *arg, struct argp_state *state) { struct test_args *args = state->input; int i; switch (key) { case ARGP_KEY_INIT: for (i = 0; state->root_argp->children[i].argp; i++) state->child_inputs[i] = args; break; case 't': args->test = 1; break; default: return ARGP_ERR_UNKNOWN; } return 0; } const char *argp_program_version = "test_argp (" PACKAGE_NAME ") " VERSION; const char *argp_program_bug_address = "<" PACKAGE_BUGREPORT ">"; static char doc[] = "documentation string"; struct argp test_argp = { main_options, parse_opt, "ARGS...", doc, NULL, NULL, NULL }; #define NARGS(a) (sizeof(a) / sizeof((a)[0]) - 1) #define ARGV0 "test-argp" #define init_args(a) memset (&(a), 0, sizeof (a)); #define INIT_TEST_COMMON(n) \ int argc = NARGS (argv); \ struct test_args test_args; \ init_args (test_args); \ test_number = n; #define INIT_TEST1(n, arg1) \ char *argv[] = { ARGV0, arg1, NULL }; \ INIT_TEST_COMMON (n) #define INIT_TEST2(n, arg1, arg2) \ char *argv[] = { ARGV0, arg1, arg2, NULL }; \ INIT_TEST_COMMON (n) #define INIT_TEST3(n, arg1, arg2, arg3) \ char *argv[] = { ARGV0, arg1, arg2, arg3, NULL }; \ INIT_TEST_COMMON (n) int test_number; unsigned failure_count = 0; void fail (const char *msg) { fprintf (stderr, "Test %d: %s\n", test_number, msg); failure_count++; } void test1 (struct argp *argp) { INIT_TEST1 (1, "--test"); if (argp_parse (argp, argc, argv, 0, NULL, &test_args)) fail ("argp_parse failed"); else if (test_args.test != 1) fail ("option not processed"); } void test2 (struct argp *argp) { INIT_TEST1 (2, "-t"); if (argp_parse (argp, argc, argv, 0, NULL, &test_args)) fail ("argp_parse failed"); else if (test_args.test != 1) fail ("option not processed"); } void test_file (struct argp *argp, int argc, char **argv, struct test_args *args) { if (argp_parse (argp, argc, argv, 0, NULL, args)) fail ("argp_parse failed"); else if (!args->file) fail ("option not processed"); else if (strcmp (args->file, "FILE")) fail ("option processed incorrectly"); } void test3 (struct argp *argp) { INIT_TEST1 (3, "--file=FILE"); test_file (argp, argc, argv, &test_args); } void test4 (struct argp *argp) { INIT_TEST2 (4, "--file", "FILE"); test_file (argp, argc, argv, &test_args); } void test5 (struct argp *argp) { INIT_TEST1 (5, "--input=FILE"); test_file (argp, argc, argv, &test_args); } void test6 (struct argp *argp) { INIT_TEST2 (6, "--input", "FILE"); test_file (argp, argc, argv, &test_args); } void test_optional (struct argp *argp, int argc, char **argv, struct test_args *args, const char *val, const char *a) { int index; if (argp_parse (argp, argc, argv, 0, &index, args)) fail ("argp_parse failed"); else if (!args->optional_set) fail ("option not processed"); if (!val) { if (args->optional) fail ("option processed incorrectly"); } else if (strcmp (args->optional, val)) fail ("option processed incorrectly"); if (a) { if (index == argc) fail ("expected command line argument not found"); else if (strcmp (argv[index], a)) fail ("expected command line argument does not match"); } } void test7 (struct argp *argp) { INIT_TEST1 (7, "-oARG"); test_optional (argp, argc, argv, &test_args, "ARG", NULL); } void test8 (struct argp *argp) { INIT_TEST2 (8, "-o", "ARG"); test_optional (argp, argc, argv, &test_args, NULL, "ARG"); } void test9 (struct argp *argp) { INIT_TEST1 (9, "--optional=ARG"); test_optional (argp, argc, argv, &test_args, "ARG", NULL); } void test10 (struct argp *argp) { INIT_TEST2 (10, "--optional", "ARG"); test_optional (argp, argc, argv, &test_args, NULL, "ARG"); } void test11 (struct argp *argp) { INIT_TEST1 (11, "--optiona=ARG"); test_optional (argp, argc, argv, &test_args, "ARG", NULL); } void test12 (struct argp *argp) { INIT_TEST3 (12, "--option", "--optional=OPT", "FILE"); test_optional (argp, argc, argv, &test_args, "OPT", "FILE"); } void test13 (struct argp *argp) { INIT_TEST1 (1, "--cantiga"); if (argp_parse (argp, argc, argv, 0, NULL, &test_args)) fail ("argp_parse failed"); else if (test_args.group_1_1_option != 'C') fail ("option not processed"); } void test14 (struct argp *argp) { INIT_TEST1 (1, "--limerick"); if (argp_parse (argp, argc, argv, 0, NULL, &test_args)) fail ("argp_parse failed"); else if (test_args.group_2_1_option != 'l') fail ("option not processed"); } void test15 (struct argp *argp) { INIT_TEST2 (1, "-r", "FILE"); test_file (argp, argc, argv, &test_args); if (!test_args.read) fail ("short alias not recognized properly"); } typedef void (*test_fp) (struct argp *argp); test_fp test_fun[] = { test1, test2, test3, test4, test5, test6, test7, test8, test9, test10, test11, test12, test13, test14, test15, NULL }; int main (int argc, char **argv) { struct argp_child argp_children[3], group1_children[2], group2_children[2]; test_fp *fun; group1_children[0] = group1_1_child; group1_children[1].argp = NULL; group1_argp.children = group1_children; group2_children[0] = group2_1_child; group2_children[1].argp = NULL; group2_argp.children = group2_children; argp_children[0] = group1_child; argp_children[1] = group2_child; argp_children[2].argp = NULL; test_argp.children = argp_children; if (argc > 0) { struct test_args test_args; init_args (test_args); return argp_parse (&test_argp, argc, argv, 0, NULL, &test_args); } for (fun = test_fun; *fun; fun++) (*fun) (&test_argp); if (failure_count) return 1; return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/test-alloca-opt.c0000644000175000017500000000276213004436755020157 00000000000000/* Test of optional automatic memory allocation. Copyright (C) 2005, 2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #if HAVE_ALLOCA static void do_allocation (int n) { void *ptr = alloca (n); (void) ptr; } void (*func) (int) = do_allocation; #endif int main () { #if HAVE_ALLOCA int i; /* Repeat a lot of times, to make sure there's no memory leak. */ for (i = 0; i < 100000; i++) { /* Try various values. n = 0 gave a crash on Alpha with gcc-2.5.8. Some versions of Mac OS X have a stack size limit of 512 KB. */ func (34); func (134); func (399); func (510823); func (129321); func (0); func (4070); func (4095); func (1); func (16582); } #endif return 0; } gnuastro-0.2.33-8a3b/bootstrapped/tests/wctomb.c0000644000175000017500000000162313004436756016436 00000000000000/* Convert wide character to multibyte character. Copyright (C) 2011-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2011. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include #include #include "wctomb-impl.h" gnuastro-0.2.33-8a3b/bootstrapped/tests/wctob.c0000644000175000017500000000226413004436756016263 00000000000000/* Convert wide character to unibyte character. Copyright (C) 2008, 2010-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2008. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include int wctob (wint_t wc) { char buf[64]; if (!(MB_CUR_MAX <= sizeof (buf))) abort (); /* Handle the case where WEOF is a value that does not fit in a wchar_t. */ if (wc == (wchar_t)wc) if (wctomb (buf, (wchar_t)wc) == 1) return (unsigned char) buf[0]; return EOF; } gnuastro-0.2.33-8a3b/bootstrapped/tests/unsetenv.c0000644000175000017500000000547213004436756017020 00000000000000/* Copyright (C) 1992, 1995-2002, 2005-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Don't use __attribute__ __nonnull__ in this compilation unit. Otherwise gcc optimizes away the name == NULL test below. */ #define _GL_ARG_NONNULL(params) #include /* Specification. */ #include #include #if !_LIBC # define __set_errno(ev) ((errno) = (ev)) #endif #include #include #if !_LIBC # define __environ environ #endif #if _LIBC /* This lock protects against simultaneous modifications of 'environ'. */ # include __libc_lock_define_initialized (static, envlock) # define LOCK __libc_lock_lock (envlock) # define UNLOCK __libc_lock_unlock (envlock) #else # define LOCK # define UNLOCK #endif /* In the GNU C library we must keep the namespace clean. */ #ifdef _LIBC # define unsetenv __unsetenv #endif #if _LIBC || !HAVE_UNSETENV int unsetenv (const char *name) { size_t len; char **ep; if (name == NULL || *name == '\0' || strchr (name, '=') != NULL) { __set_errno (EINVAL); return -1; } len = strlen (name); LOCK; ep = __environ; while (*ep != NULL) if (!strncmp (*ep, name, len) && (*ep)[len] == '=') { /* Found it. Remove this pointer by moving later ones back. */ char **dp = ep; do dp[0] = dp[1]; while (*dp++); /* Continue the loop in case NAME appears again. */ } else ++ep; UNLOCK; return 0; } #ifdef _LIBC # undef unsetenv weak_alias (__unsetenv, unsetenv) #endif #else /* HAVE_UNSETENV */ # undef unsetenv # if !HAVE_DECL_UNSETENV # if VOID_UNSETENV extern void unsetenv (const char *); # else extern int unsetenv (const char *); # endif # endif /* Call the underlying unsetenv, in case there is hidden bookkeeping that needs updating beyond just modifying environ. */ int rpl_unsetenv (const char *name) { int result = 0; if (!name || !*name || strchr (name, '=')) { errno = EINVAL; return -1; } while (getenv (name)) # if !VOID_UNSETENV result = # endif unsetenv (name); return result; } #endif /* HAVE_UNSETENV */ gnuastro-0.2.33-8a3b/bootstrapped/tests/symlink.c0000644000175000017500000000263113004436755016630 00000000000000/* Stub for symlink(). Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include #include #if HAVE_SYMLINK # undef symlink /* Create a symlink, but reject trailing slash. */ int rpl_symlink (char const *contents, char const *name) { size_t len = strlen (name); if (len && name[len - 1] == '/') { struct stat st; if (lstat (name, &st) == 0) errno = EEXIST; return -1; } return symlink (contents, name); } #else /* !HAVE_SYMLINK */ /* The system does not support symlinks. */ int symlink (char const *contents _GL_UNUSED, char const *name _GL_UNUSED) { errno = ENOSYS; return -1; } #endif /* !HAVE_SYMLINK */ gnuastro-0.2.33-8a3b/bootstrapped/tests/stat.c0000644000175000017500000001066613004436755016124 00000000000000/* Work around platform bugs in stat. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* written by Eric Blake */ /* If the user's config.h happens to include , let it include only the system's here, so that orig_stat doesn't recurse to rpl_stat. */ #define __need_system_sys_stat_h #include /* Get the original definition of stat. It might be defined as a macro. */ #include #include #undef __need_system_sys_stat_h #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # if _GL_WINDOWS_64_BIT_ST_SIZE # undef stat /* avoid warning on mingw64 with _FILE_OFFSET_BITS=64 */ # define stat _stati64 # define REPLACE_FUNC_STAT_DIR 1 # undef REPLACE_FUNC_STAT_FILE # elif REPLACE_FUNC_STAT_FILE /* mingw64 has a broken stat() function, based on _stat(), in libmingwex.a. Bypass it. */ # define stat _stat # define REPLACE_FUNC_STAT_DIR 1 # undef REPLACE_FUNC_STAT_FILE # endif #endif static int orig_stat (const char *filename, struct stat *buf) { return stat (filename, buf); } /* Specification. */ /* Write "sys/stat.h" here, not , otherwise OSF/1 5.1 DTK cc eliminates this include because of the preliminary #include above. */ #include "sys/stat.h" #include #include #include #include #include "dosname.h" #include "verify.h" #if REPLACE_FUNC_STAT_DIR # include "pathmax.h" /* The only known systems where REPLACE_FUNC_STAT_DIR is needed also have a constant PATH_MAX. */ # ifndef PATH_MAX # error "Please port this replacement to your platform" # endif #endif /* Store information about NAME into ST. Work around bugs with trailing slashes. Mingw has other bugs (such as st_ino always being 0 on success) which this wrapper does not work around. But at least this implementation provides the ability to emulate fchdir correctly. */ int rpl_stat (char const *name, struct stat *st) { int result = orig_stat (name, st); #if REPLACE_FUNC_STAT_FILE /* Solaris 9 mistakenly succeeds when given a non-directory with a trailing slash. */ if (result == 0 && !S_ISDIR (st->st_mode)) { size_t len = strlen (name); if (ISSLASH (name[len - 1])) { errno = ENOTDIR; return -1; } } #endif /* REPLACE_FUNC_STAT_FILE */ #if REPLACE_FUNC_STAT_DIR if (result == -1 && errno == ENOENT) { /* Due to mingw's oddities, there are some directories (like c:\) where stat() only succeeds with a trailing slash, and other directories (like c:\windows) where stat() only succeeds without a trailing slash. But we want the two to be synonymous, since chdir() manages either style. Likewise, Mingw also reports ENOENT for names longer than PATH_MAX, when we want ENAMETOOLONG, and for stat("file/"), when we want ENOTDIR. Fortunately, mingw PATH_MAX is small enough for stack allocation. */ char fixed_name[PATH_MAX + 1] = {0}; size_t len = strlen (name); bool check_dir = false; verify (PATH_MAX <= 4096); if (PATH_MAX <= len) errno = ENAMETOOLONG; else if (len) { strcpy (fixed_name, name); if (ISSLASH (fixed_name[len - 1])) { check_dir = true; while (len && ISSLASH (fixed_name[len - 1])) fixed_name[--len] = '\0'; if (!len) fixed_name[0] = '/'; } else fixed_name[len++] = '/'; result = orig_stat (fixed_name, st); if (result == 0 && check_dir && !S_ISDIR (st->st_mode)) { result = -1; errno = ENOTDIR; } } } #endif /* REPLACE_FUNC_STAT_DIR */ return result; } gnuastro-0.2.33-8a3b/bootstrapped/tests/setlocale.c0000644000175000017500000007007413004436755017123 00000000000000/* Set the current locale. -*- coding: utf-8 -*- Copyright (C) 2009, 2011-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ #include /* Override setlocale() so that when the default locale is requested (locale = ""), the environment variables LC_ALL, LC_*, and LANG are considered. Also include all the functionality from libintl's setlocale() override. */ /* Please keep this file in sync with gettext/gettext-runtime/intl/setlocale.c ! */ /* Specification. */ #include #include #include #include "localename.h" #if 1 # undef setlocale /* Return string representation of locale category CATEGORY. */ static const char * category_to_name (int category) { const char *retval; switch (category) { case LC_COLLATE: retval = "LC_COLLATE"; break; case LC_CTYPE: retval = "LC_CTYPE"; break; case LC_MONETARY: retval = "LC_MONETARY"; break; case LC_NUMERIC: retval = "LC_NUMERIC"; break; case LC_TIME: retval = "LC_TIME"; break; case LC_MESSAGES: retval = "LC_MESSAGES"; break; default: /* If you have a better idea for a default value let me know. */ retval = "LC_XXX"; } return retval; } # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* The native Windows setlocale() function expects locale names of the form "German" or "German_Germany" or "DEU", but not "de" or "de_DE". We need to convert the names from the form with ISO 639 language code and ISO 3166 country code to the form with English names or with three-letter identifier. The three-letter identifiers known by a Windows XP SP2 or SP3 are: AFK Afrikaans_South Africa.1252 ARA Arabic_Saudi Arabia.1256 ARB Arabic_Lebanon.1256 ARE Arabic_Egypt.1256 ARG Arabic_Algeria.1256 ARH Arabic_Bahrain.1256 ARI Arabic_Iraq.1256 ARJ Arabic_Jordan.1256 ARK Arabic_Kuwait.1256 ARL Arabic_Libya.1256 ARM Arabic_Morocco.1256 ARO Arabic_Oman.1256 ARQ Arabic_Qatar.1256 ARS Arabic_Syria.1256 ART Arabic_Tunisia.1256 ARU Arabic_U.A.E..1256 ARY Arabic_Yemen.1256 AZE Azeri (Latin)_Azerbaijan.1254 BEL Belarusian_Belarus.1251 BGR Bulgarian_Bulgaria.1251 BSB Bosnian_Bosnia and Herzegovina.1250 BSC Bosnian (Cyrillic)_Bosnia and Herzegovina.1250 (wrong encoding!) CAT Catalan_Spain.1252 CHH Chinese_Hong Kong S.A.R..950 CHI Chinese_Singapore.936 CHS Chinese_People's Republic of China.936 CHT Chinese_Taiwan.950 CSY Czech_Czech Republic.1250 CYM Welsh_United Kingdom.1252 DAN Danish_Denmark.1252 DEA German_Austria.1252 DEC German_Liechtenstein.1252 DEL German_Luxembourg.1252 DES German_Switzerland.1252 DEU German_Germany.1252 ELL Greek_Greece.1253 ENA English_Australia.1252 ENB English_Caribbean.1252 ENC English_Canada.1252 ENG English_United Kingdom.1252 ENI English_Ireland.1252 ENJ English_Jamaica.1252 ENL English_Belize.1252 ENP English_Republic of the Philippines.1252 ENS English_South Africa.1252 ENT English_Trinidad and Tobago.1252 ENU English_United States.1252 ENW English_Zimbabwe.1252 ENZ English_New Zealand.1252 ESA Spanish_Panama.1252 ESB Spanish_Bolivia.1252 ESC Spanish_Costa Rica.1252 ESD Spanish_Dominican Republic.1252 ESE Spanish_El Salvador.1252 ESF Spanish_Ecuador.1252 ESG Spanish_Guatemala.1252 ESH Spanish_Honduras.1252 ESI Spanish_Nicaragua.1252 ESL Spanish_Chile.1252 ESM Spanish_Mexico.1252 ESN Spanish_Spain.1252 ESO Spanish_Colombia.1252 ESP Spanish_Spain.1252 ESR Spanish_Peru.1252 ESS Spanish_Argentina.1252 ESU Spanish_Puerto Rico.1252 ESV Spanish_Venezuela.1252 ESY Spanish_Uruguay.1252 ESZ Spanish_Paraguay.1252 ETI Estonian_Estonia.1257 EUQ Basque_Spain.1252 FAR Farsi_Iran.1256 FIN Finnish_Finland.1252 FOS Faroese_Faroe Islands.1252 FPO Filipino_Philippines.1252 FRA French_France.1252 FRB French_Belgium.1252 FRC French_Canada.1252 FRL French_Luxembourg.1252 FRM French_Principality of Monaco.1252 FRS French_Switzerland.1252 FYN Frisian_Netherlands.1252 GLC Galician_Spain.1252 HEB Hebrew_Israel.1255 HRB Croatian_Bosnia and Herzegovina.1250 HRV Croatian_Croatia.1250 HUN Hungarian_Hungary.1250 IND Indonesian_Indonesia.1252 IRE Irish_Ireland.1252 ISL Icelandic_Iceland.1252 ITA Italian_Italy.1252 ITS Italian_Switzerland.1252 IUK Inuktitut (Latin)_Canada.1252 JPN Japanese_Japan.932 KKZ Kazakh_Kazakhstan.1251 KOR Korean_Korea.949 KYR Kyrgyz_Kyrgyzstan.1251 LBX Luxembourgish_Luxembourg.1252 LTH Lithuanian_Lithuania.1257 LVI Latvian_Latvia.1257 MKI FYRO Macedonian_Former Yugoslav Republic of Macedonia.1251 MON Mongolian_Mongolia.1251 MPD Mapudungun_Chile.1252 MSB Malay_Brunei Darussalam.1252 MSL Malay_Malaysia.1252 MWK Mohawk_Canada.1252 NLB Dutch_Belgium.1252 NLD Dutch_Netherlands.1252 NON Norwegian-Nynorsk_Norway.1252 NOR Norwegian (BokmÃ¥l)_Norway.1252 NSO Northern Sotho_South Africa.1252 PLK Polish_Poland.1250 PTB Portuguese_Brazil.1252 PTG Portuguese_Portugal.1252 QUB Quechua_Bolivia.1252 QUE Quechua_Ecuador.1252 QUP Quechua_Peru.1252 RMC Romansh_Switzerland.1252 ROM Romanian_Romania.1250 RUS Russian_Russia.1251 SKY Slovak_Slovakia.1250 SLV Slovenian_Slovenia.1250 SMA Sami (Southern)_Norway.1252 SMB Sami (Southern)_Sweden.1252 SME Sami (Northern)_Norway.1252 SMF Sami (Northern)_Sweden.1252 SMG Sami (Northern)_Finland.1252 SMJ Sami (Lule)_Norway.1252 SMK Sami (Lule)_Sweden.1252 SMN Sami (Inari)_Finland.1252 SMS Sami (Skolt)_Finland.1252 SQI Albanian_Albania.1250 SRB Serbian (Cyrillic)_Serbia and Montenegro.1251 SRL Serbian (Latin)_Serbia and Montenegro.1250 SRN Serbian (Cyrillic)_Bosnia and Herzegovina.1251 SRS Serbian (Latin)_Bosnia and Herzegovina.1250 SVE Swedish_Sweden.1252 SVF Swedish_Finland.1252 SWK Swahili_Kenya.1252 THA Thai_Thailand.874 TRK Turkish_Turkey.1254 TSN Tswana_South Africa.1252 TTT Tatar_Russia.1251 UKR Ukrainian_Ukraine.1251 URD Urdu_Islamic Republic of Pakistan.1256 USA English_United States.1252 UZB Uzbek (Latin)_Uzbekistan.1254 VIT Vietnamese_Viet Nam.1258 XHO Xhosa_South Africa.1252 ZHH Chinese_Hong Kong S.A.R..950 ZHI Chinese_Singapore.936 ZHM Chinese_Macau S.A.R..950 ZUL Zulu_South Africa.1252 */ /* Table from ISO 639 language code, optionally with country or script suffix, to English name. Keep in sync with the gl_locale_name_from_win32_LANGID function in localename.c! */ struct table_entry { const char *code; const char *english; }; static const struct table_entry language_table[] = { { "af", "Afrikaans" }, { "am", "Amharic" }, { "ar", "Arabic" }, { "arn", "Mapudungun" }, { "as", "Assamese" }, { "az@cyrillic", "Azeri (Cyrillic)" }, { "az@latin", "Azeri (Latin)" }, { "ba", "Bashkir" }, { "be", "Belarusian" }, { "ber", "Tamazight" }, { "ber@arabic", "Tamazight (Arabic)" }, { "ber@latin", "Tamazight (Latin)" }, { "bg", "Bulgarian" }, { "bin", "Edo" }, { "bn", "Bengali" }, { "bn_BD", "Bengali (Bangladesh)" }, { "bn_IN", "Bengali (India)" }, { "bnt", "Sutu" }, { "bo", "Tibetan" }, { "br", "Breton" }, { "bs", "BSB" }, /* "Bosnian (Latin)" */ { "bs@cyrillic", "BSC" }, /* Bosnian (Cyrillic) */ { "ca", "Catalan" }, { "chr", "Cherokee" }, { "co", "Corsican" }, { "cpe", "Hawaiian" }, { "cs", "Czech" }, { "cy", "Welsh" }, { "da", "Danish" }, { "de", "German" }, { "dsb", "Lower Sorbian" }, { "dv", "Divehi" }, { "el", "Greek" }, { "en", "English" }, { "es", "Spanish" }, { "et", "Estonian" }, { "eu", "Basque" }, { "fa", "Farsi" }, { "ff", "Fulfulde" }, { "fi", "Finnish" }, { "fo", "Faroese" }, /* "Faeroese" does not work */ { "fr", "French" }, { "fy", "Frisian" }, { "ga", "IRE" }, /* Gaelic (Ireland) */ { "gd", "Gaelic (Scotland)" }, { "gd", "Scottish Gaelic" }, { "gl", "Galician" }, { "gn", "Guarani" }, { "gsw", "Alsatian" }, { "gu", "Gujarati" }, { "ha", "Hausa" }, { "he", "Hebrew" }, { "hi", "Hindi" }, { "hr", "Croatian" }, { "hsb", "Upper Sorbian" }, { "hu", "Hungarian" }, { "hy", "Armenian" }, { "id", "Indonesian" }, { "ig", "Igbo" }, { "ii", "Yi" }, { "is", "Icelandic" }, { "it", "Italian" }, { "iu", "IUK" }, /* Inuktitut */ { "ja", "Japanese" }, { "ka", "Georgian" }, { "kk", "Kazakh" }, { "kl", "Greenlandic" }, { "km", "Cambodian" }, { "km", "Khmer" }, { "kn", "Kannada" }, { "ko", "Korean" }, { "kok", "Konkani" }, { "kr", "Kanuri" }, { "ks", "Kashmiri" }, { "ks_IN", "Kashmiri_India" }, { "ks_PK", "Kashmiri (Arabic)_Pakistan" }, { "ky", "Kyrgyz" }, { "la", "Latin" }, { "lb", "Luxembourgish" }, { "lo", "Lao" }, { "lt", "Lithuanian" }, { "lv", "Latvian" }, { "mi", "Maori" }, { "mk", "FYRO Macedonian" }, { "mk", "Macedonian" }, { "ml", "Malayalam" }, { "mn", "Mongolian" }, { "mni", "Manipuri" }, { "moh", "Mohawk" }, { "mr", "Marathi" }, { "ms", "Malay" }, { "mt", "Maltese" }, { "my", "Burmese" }, { "nb", "NOR" }, /* Norwegian BokmÃ¥l */ { "ne", "Nepali" }, { "nic", "Ibibio" }, { "nl", "Dutch" }, { "nn", "NON" }, /* Norwegian Nynorsk */ { "no", "Norwegian" }, { "nso", "Northern Sotho" }, { "nso", "Sepedi" }, { "oc", "Occitan" }, { "om", "Oromo" }, { "or", "Oriya" }, { "pa", "Punjabi" }, { "pap", "Papiamentu" }, { "pl", "Polish" }, { "prs", "Dari" }, { "ps", "Pashto" }, { "pt", "Portuguese" }, { "qu", "Quechua" }, { "qut", "K'iche'" }, { "rm", "Romansh" }, { "ro", "Romanian" }, { "ru", "Russian" }, { "rw", "Kinyarwanda" }, { "sa", "Sanskrit" }, { "sah", "Yakut" }, { "sd", "Sindhi" }, { "se", "Sami (Northern)" }, { "se", "Northern Sami" }, { "si", "Sinhalese" }, { "sk", "Slovak" }, { "sl", "Slovenian" }, { "sma", "Sami (Southern)" }, { "sma", "Southern Sami" }, { "smj", "Sami (Lule)" }, { "smj", "Lule Sami" }, { "smn", "Sami (Inari)" }, { "smn", "Inari Sami" }, { "sms", "Sami (Skolt)" }, { "sms", "Skolt Sami" }, { "so", "Somali" }, { "sq", "Albanian" }, { "sr", "Serbian (Latin)" }, { "sr@cyrillic", "SRB" }, /* Serbian (Cyrillic) */ { "sv", "Swedish" }, { "sw", "Swahili" }, { "syr", "Syriac" }, { "ta", "Tamil" }, { "te", "Telugu" }, { "tg", "Tajik" }, { "th", "Thai" }, { "ti", "Tigrinya" }, { "tk", "Turkmen" }, { "tl", "Filipino" }, { "tn", "Tswana" }, { "tr", "Turkish" }, { "ts", "Tsonga" }, { "tt", "Tatar" }, { "ug", "Uighur" }, { "uk", "Ukrainian" }, { "ur", "Urdu" }, { "uz", "Uzbek" }, { "uz", "Uzbek (Latin)" }, { "uz@cyrillic", "Uzbek (Cyrillic)" }, { "ve", "Venda" }, { "vi", "Vietnamese" }, { "wen", "Sorbian" }, { "wo", "Wolof" }, { "xh", "Xhosa" }, { "yi", "Yiddish" }, { "yo", "Yoruba" }, { "zh", "Chinese" }, { "zu", "Zulu" } }; /* Table from ISO 3166 country code to English name. Keep in sync with the gl_locale_name_from_win32_LANGID function in localename.c! */ static const struct table_entry country_table[] = { { "AE", "U.A.E." }, { "AF", "Afghanistan" }, { "AL", "Albania" }, { "AM", "Armenia" }, { "AN", "Netherlands Antilles" }, { "AR", "Argentina" }, { "AT", "Austria" }, { "AU", "Australia" }, { "AZ", "Azerbaijan" }, { "BA", "Bosnia and Herzegovina" }, { "BD", "Bangladesh" }, { "BE", "Belgium" }, { "BG", "Bulgaria" }, { "BH", "Bahrain" }, { "BN", "Brunei Darussalam" }, { "BO", "Bolivia" }, { "BR", "Brazil" }, { "BT", "Bhutan" }, { "BY", "Belarus" }, { "BZ", "Belize" }, { "CA", "Canada" }, { "CG", "Congo" }, { "CH", "Switzerland" }, { "CI", "Cote d'Ivoire" }, { "CL", "Chile" }, { "CM", "Cameroon" }, { "CN", "People's Republic of China" }, { "CO", "Colombia" }, { "CR", "Costa Rica" }, { "CS", "Serbia and Montenegro" }, { "CZ", "Czech Republic" }, { "DE", "Germany" }, { "DK", "Denmark" }, { "DO", "Dominican Republic" }, { "DZ", "Algeria" }, { "EC", "Ecuador" }, { "EE", "Estonia" }, { "EG", "Egypt" }, { "ER", "Eritrea" }, { "ES", "Spain" }, { "ET", "Ethiopia" }, { "FI", "Finland" }, { "FO", "Faroe Islands" }, { "FR", "France" }, { "GB", "United Kingdom" }, { "GD", "Caribbean" }, { "GE", "Georgia" }, { "GL", "Greenland" }, { "GR", "Greece" }, { "GT", "Guatemala" }, { "HK", "Hong Kong" }, { "HK", "Hong Kong S.A.R." }, { "HN", "Honduras" }, { "HR", "Croatia" }, { "HT", "Haiti" }, { "HU", "Hungary" }, { "ID", "Indonesia" }, { "IE", "Ireland" }, { "IL", "Israel" }, { "IN", "India" }, { "IQ", "Iraq" }, { "IR", "Iran" }, { "IS", "Iceland" }, { "IT", "Italy" }, { "JM", "Jamaica" }, { "JO", "Jordan" }, { "JP", "Japan" }, { "KE", "Kenya" }, { "KG", "Kyrgyzstan" }, { "KH", "Cambodia" }, { "KR", "South Korea" }, { "KW", "Kuwait" }, { "KZ", "Kazakhstan" }, { "LA", "Laos" }, { "LB", "Lebanon" }, { "LI", "Liechtenstein" }, { "LK", "Sri Lanka" }, { "LT", "Lithuania" }, { "LU", "Luxembourg" }, { "LV", "Latvia" }, { "LY", "Libya" }, { "MA", "Morocco" }, { "MC", "Principality of Monaco" }, { "MD", "Moldava" }, { "MD", "Moldova" }, { "ME", "Montenegro" }, { "MK", "Former Yugoslav Republic of Macedonia" }, { "ML", "Mali" }, { "MM", "Myanmar" }, { "MN", "Mongolia" }, { "MO", "Macau S.A.R." }, { "MT", "Malta" }, { "MV", "Maldives" }, { "MX", "Mexico" }, { "MY", "Malaysia" }, { "NG", "Nigeria" }, { "NI", "Nicaragua" }, { "NL", "Netherlands" }, { "NO", "Norway" }, { "NP", "Nepal" }, { "NZ", "New Zealand" }, { "OM", "Oman" }, { "PA", "Panama" }, { "PE", "Peru" }, { "PH", "Philippines" }, { "PK", "Islamic Republic of Pakistan" }, { "PL", "Poland" }, { "PR", "Puerto Rico" }, { "PT", "Portugal" }, { "PY", "Paraguay" }, { "QA", "Qatar" }, { "RE", "Reunion" }, { "RO", "Romania" }, { "RS", "Serbia" }, { "RU", "Russia" }, { "RW", "Rwanda" }, { "SA", "Saudi Arabia" }, { "SE", "Sweden" }, { "SG", "Singapore" }, { "SI", "Slovenia" }, { "SK", "Slovak" }, { "SN", "Senegal" }, { "SO", "Somalia" }, { "SR", "Suriname" }, { "SV", "El Salvador" }, { "SY", "Syria" }, { "TH", "Thailand" }, { "TJ", "Tajikistan" }, { "TM", "Turkmenistan" }, { "TN", "Tunisia" }, { "TR", "Turkey" }, { "TT", "Trinidad and Tobago" }, { "TW", "Taiwan" }, { "TZ", "Tanzania" }, { "UA", "Ukraine" }, { "US", "United States" }, { "UY", "Uruguay" }, { "VA", "Vatican" }, { "VE", "Venezuela" }, { "VN", "Viet Nam" }, { "YE", "Yemen" }, { "ZA", "South Africa" }, { "ZW", "Zimbabwe" } }; /* Given a string STRING, find the set of indices i such that TABLE[i].code is the given STRING. It is a range [lo,hi-1]. */ typedef struct { size_t lo; size_t hi; } range_t; static void search (const struct table_entry *table, size_t table_size, const char *string, range_t *result) { /* The table is sorted. Perform a binary search. */ size_t hi = table_size; size_t lo = 0; while (lo < hi) { /* Invariant: for i < lo, strcmp (table[i].code, string) < 0, for i >= hi, strcmp (table[i].code, string) > 0. */ size_t mid = (hi + lo) >> 1; /* >= lo, < hi */ int cmp = strcmp (table[mid].code, string); if (cmp < 0) lo = mid + 1; else if (cmp > 0) hi = mid; else { /* Found an i with strcmp (language_table[i].code, string) == 0. Find the entire interval of such i. */ { size_t i; for (i = mid; i > lo; ) { i--; if (strcmp (table[i].code, string) < 0) { lo = i + 1; break; } } } { size_t i; for (i = mid; i < hi; i++) { if (strcmp (table[i].code, string) > 0) { hi = i; break; } } } /* The set of i with strcmp (language_table[i].code, string) == 0 is the interval [lo, hi-1]. */ break; } } result->lo = lo; result->hi = hi; } /* Like setlocale, but accept also locale names in the form ll or ll_CC, where ll is an ISO 639 language code and CC is an ISO 3166 country code. */ static char * setlocale_unixlike (int category, const char *locale) { char *result; char llCC_buf[64]; char ll_buf[64]; char CC_buf[64]; /* First, try setlocale with the original argument unchanged. */ result = setlocale (category, locale); if (result != NULL) return result; /* Otherwise, assume the argument is in the form language[_territory][.codeset][@modifier] and try to map it using the tables. */ if (strlen (locale) < sizeof (llCC_buf)) { /* Second try: Remove the codeset part. */ { const char *p = locale; char *q = llCC_buf; /* Copy the part before the dot. */ for (; *p != '\0' && *p != '.'; p++, q++) *q = *p; if (*p == '.') /* Skip the part up to the '@', if any. */ for (; *p != '\0' && *p != '@'; p++) ; /* Copy the part starting with '@', if any. */ for (; *p != '\0'; p++, q++) *q = *p; *q = '\0'; } /* llCC_buf now contains language[_territory][@modifier] */ if (strcmp (llCC_buf, locale) != 0) { result = setlocale (category, llCC_buf); if (result != NULL) return result; } /* Look it up in language_table. */ { range_t range; size_t i; search (language_table, sizeof (language_table) / sizeof (language_table[0]), llCC_buf, &range); for (i = range.lo; i < range.hi; i++) { /* Try the replacement in language_table[i]. */ result = setlocale (category, language_table[i].english); if (result != NULL) return result; } } /* Split language[_territory][@modifier] into ll_buf = language[@modifier] and CC_buf = territory */ { const char *underscore = strchr (llCC_buf, '_'); if (underscore != NULL) { const char *territory_start = underscore + 1; const char *territory_end = strchr (territory_start, '@'); if (territory_end == NULL) territory_end = territory_start + strlen (territory_start); memcpy (ll_buf, llCC_buf, underscore - llCC_buf); strcpy (ll_buf + (underscore - llCC_buf), territory_end); memcpy (CC_buf, territory_start, territory_end - territory_start); CC_buf[territory_end - territory_start] = '\0'; { /* Look up ll_buf in language_table and CC_buf in country_table. */ range_t language_range; search (language_table, sizeof (language_table) / sizeof (language_table[0]), ll_buf, &language_range); if (language_range.lo < language_range.hi) { range_t country_range; search (country_table, sizeof (country_table) / sizeof (country_table[0]), CC_buf, &country_range); if (country_range.lo < country_range.hi) { size_t i; size_t j; for (i = language_range.lo; i < language_range.hi; i++) for (j = country_range.lo; j < country_range.hi; j++) { /* Concatenate the replacements. */ const char *part1 = language_table[i].english; size_t part1_len = strlen (part1); const char *part2 = country_table[j].english; size_t part2_len = strlen (part2) + 1; char buf[64+64]; if (!(part1_len + 1 + part2_len <= sizeof (buf))) abort (); memcpy (buf, part1, part1_len); buf[part1_len] = '_'; memcpy (buf + part1_len + 1, part2, part2_len); /* Try the concatenated replacements. */ result = setlocale (category, buf); if (result != NULL) return result; } } /* Try omitting the country entirely. This may set a locale corresponding to the wrong country, but is better than failing entirely. */ { size_t i; for (i = language_range.lo; i < language_range.hi; i++) { /* Try only the language replacement. */ result = setlocale (category, language_table[i].english); if (result != NULL) return result; } } } } } } } /* Failed. */ return NULL; } # else # define setlocale_unixlike setlocale # endif # if LC_MESSAGES == 1729 /* The system does not store an LC_MESSAGES locale category. Do it here. */ static char lc_messages_name[64] = "C"; /* Like setlocale, but support also LC_MESSAGES. */ static char * setlocale_single (int category, const char *locale) { if (category == LC_MESSAGES) { if (locale != NULL) { lc_messages_name[sizeof (lc_messages_name) - 1] = '\0'; strncpy (lc_messages_name, locale, sizeof (lc_messages_name) - 1); } return lc_messages_name; } else return setlocale_unixlike (category, locale); } # else # define setlocale_single setlocale_unixlike # endif char * rpl_setlocale (int category, const char *locale) { if (locale != NULL && locale[0] == '\0') { /* A request to the set the current locale to the default locale. */ if (category == LC_ALL) { /* Set LC_CTYPE first. Then the other categories. */ static int const categories[] = { LC_NUMERIC, LC_TIME, LC_COLLATE, LC_MONETARY, LC_MESSAGES }; char *saved_locale; const char *base_name; unsigned int i; /* Back up the old locale, in case one of the steps fails. */ saved_locale = setlocale (LC_ALL, NULL); if (saved_locale == NULL) return NULL; saved_locale = strdup (saved_locale); if (saved_locale == NULL) return NULL; /* Set LC_CTYPE category. Set all other categories (except possibly LC_MESSAGES) to the same value in the same call; this is likely to save calls. */ base_name = gl_locale_name_environ (LC_CTYPE, category_to_name (LC_CTYPE)); if (base_name == NULL) base_name = gl_locale_name_default (); if (setlocale_unixlike (LC_ALL, base_name) == NULL) goto fail; # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* On native Windows, setlocale(LC_ALL,...) may succeed but set the LC_CTYPE category to an invalid value ("C") when it does not support the specified encoding. Report a failure instead. */ if (strchr (base_name, '.') != NULL && strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) goto fail; # endif for (i = 0; i < sizeof (categories) / sizeof (categories[0]); i++) { int cat = categories[i]; const char *name; name = gl_locale_name_environ (cat, category_to_name (cat)); if (name == NULL) name = gl_locale_name_default (); /* If name is the same as base_name, it has already been set through the setlocale call before the loop. */ if (strcmp (name, base_name) != 0 # if LC_MESSAGES == 1729 || cat == LC_MESSAGES # endif ) if (setlocale_single (cat, name) == NULL) goto fail; } /* All steps were successful. */ free (saved_locale); return setlocale (LC_ALL, NULL); fail: if (saved_locale[0] != '\0') /* don't risk an endless recursion */ setlocale (LC_ALL, saved_locale); free (saved_locale); return NULL; } else { const char *name = gl_locale_name_environ (category, category_to_name (category)); if (name == NULL) name = gl_locale_name_default (); return setlocale_single (category, name); } } else { # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ if (category == LC_ALL && locale != NULL && strchr (locale, '.') != NULL) { char *saved_locale; /* Back up the old locale. */ saved_locale = setlocale (LC_ALL, NULL); if (saved_locale == NULL) return NULL; saved_locale = strdup (saved_locale); if (saved_locale == NULL) return NULL; if (setlocale_unixlike (LC_ALL, locale) == NULL) { free (saved_locale); return NULL; } /* On native Windows, setlocale(LC_ALL,...) may succeed but set the LC_CTYPE category to an invalid value ("C") when it does not support the specified encoding. Report a failure instead. */ if (strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) { if (saved_locale[0] != '\0') /* don't risk an endless recursion */ setlocale (LC_ALL, saved_locale); free (saved_locale); return NULL; } /* It was really successful. */ free (saved_locale); return setlocale (LC_ALL, NULL); } else # endif return setlocale_single (category, locale); } } #endif gnuastro-0.2.33-8a3b/bootstrapped/tests/setenv.c0000644000175000017500000002502613004436755016451 00000000000000/* Copyright (C) 1992, 1995-2003, 2005-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #if !_LIBC /* Don't use __attribute__ __nonnull__ in this compilation unit. Otherwise gcc optimizes away the name == NULL test below. */ # define _GL_ARG_NONNULL(params) # define _GL_USE_STDLIB_ALLOC 1 # include #endif #include /* Specification. */ #include #include #ifndef __set_errno # define __set_errno(ev) ((errno) = (ev)) #endif #include #if _LIBC || HAVE_UNISTD_H # include #endif #if !_LIBC # include "malloca.h" #endif #if _LIBC || !HAVE_SETENV #if !_LIBC # define __environ environ #endif #if _LIBC /* This lock protects against simultaneous modifications of 'environ'. */ # include __libc_lock_define_initialized (static, envlock) # define LOCK __libc_lock_lock (envlock) # define UNLOCK __libc_lock_unlock (envlock) #else # define LOCK # define UNLOCK #endif /* In the GNU C library we must keep the namespace clean. */ #ifdef _LIBC # define setenv __setenv # define clearenv __clearenv # define tfind __tfind # define tsearch __tsearch #endif /* In the GNU C library implementation we try to be more clever and allow arbitrarily many changes of the environment given that the used values are from a small set. Outside glibc this will eat up all memory after a while. */ #if defined _LIBC || (defined HAVE_SEARCH_H && defined HAVE_TSEARCH \ && defined __GNUC__) # define USE_TSEARCH 1 # include typedef int (*compar_fn_t) (const void *, const void *); /* This is a pointer to the root of the search tree with the known values. */ static void *known_values; # define KNOWN_VALUE(Str) \ ({ \ void *value = tfind (Str, &known_values, (compar_fn_t) strcmp); \ value != NULL ? *(char **) value : NULL; \ }) # define STORE_VALUE(Str) \ tsearch (Str, &known_values, (compar_fn_t) strcmp) #else # undef USE_TSEARCH # define KNOWN_VALUE(Str) NULL # define STORE_VALUE(Str) do { } while (0) #endif /* If this variable is not a null pointer we allocated the current environment. */ static char **last_environ; /* This function is used by 'setenv' and 'putenv'. The difference between the two functions is that for the former must create a new string which is then placed in the environment, while the argument of 'putenv' must be used directly. This is all complicated by the fact that we try to reuse values once generated for a 'setenv' call since we can never free the strings. */ int __add_to_environ (const char *name, const char *value, const char *combined, int replace) { char **ep; size_t size; const size_t namelen = strlen (name); const size_t vallen = value != NULL ? strlen (value) + 1 : 0; LOCK; /* We have to get the pointer now that we have the lock and not earlier since another thread might have created a new environment. */ ep = __environ; size = 0; if (ep != NULL) { for (; *ep != NULL; ++ep) if (!strncmp (*ep, name, namelen) && (*ep)[namelen] == '=') break; else ++size; } if (ep == NULL || *ep == NULL) { char **new_environ; #ifdef USE_TSEARCH char *new_value; #endif /* We allocated this space; we can extend it. */ new_environ = (char **) (last_environ == NULL ? malloc ((size + 2) * sizeof (char *)) : realloc (last_environ, (size + 2) * sizeof (char *))); if (new_environ == NULL) { /* It's easier to set errno to ENOMEM than to rely on the 'malloc-posix' and 'realloc-posix' gnulib modules. */ __set_errno (ENOMEM); UNLOCK; return -1; } /* If the whole entry is given add it. */ if (combined != NULL) /* We must not add the string to the search tree since it belongs to the user. */ new_environ[size] = (char *) combined; else { /* See whether the value is already known. */ #ifdef USE_TSEARCH # ifdef _LIBC new_value = (char *) alloca (namelen + 1 + vallen); __mempcpy (__mempcpy (__mempcpy (new_value, name, namelen), "=", 1), value, vallen); # else new_value = (char *) malloca (namelen + 1 + vallen); if (new_value == NULL) { __set_errno (ENOMEM); UNLOCK; return -1; } memcpy (new_value, name, namelen); new_value[namelen] = '='; memcpy (&new_value[namelen + 1], value, vallen); # endif new_environ[size] = KNOWN_VALUE (new_value); if (new_environ[size] == NULL) #endif { new_environ[size] = (char *) malloc (namelen + 1 + vallen); if (new_environ[size] == NULL) { #if defined USE_TSEARCH && !defined _LIBC freea (new_value); #endif __set_errno (ENOMEM); UNLOCK; return -1; } #ifdef USE_TSEARCH memcpy (new_environ[size], new_value, namelen + 1 + vallen); #else memcpy (new_environ[size], name, namelen); new_environ[size][namelen] = '='; memcpy (&new_environ[size][namelen + 1], value, vallen); #endif /* And save the value now. We cannot do this when we remove the string since then we cannot decide whether it is a user string or not. */ STORE_VALUE (new_environ[size]); } #if defined USE_TSEARCH && !defined _LIBC freea (new_value); #endif } if (__environ != last_environ) memcpy ((char *) new_environ, (char *) __environ, size * sizeof (char *)); new_environ[size + 1] = NULL; last_environ = __environ = new_environ; } else if (replace) { char *np; /* Use the user string if given. */ if (combined != NULL) np = (char *) combined; else { #ifdef USE_TSEARCH char *new_value; # ifdef _LIBC new_value = alloca (namelen + 1 + vallen); __mempcpy (__mempcpy (__mempcpy (new_value, name, namelen), "=", 1), value, vallen); # else new_value = malloca (namelen + 1 + vallen); if (new_value == NULL) { __set_errno (ENOMEM); UNLOCK; return -1; } memcpy (new_value, name, namelen); new_value[namelen] = '='; memcpy (&new_value[namelen + 1], value, vallen); # endif np = KNOWN_VALUE (new_value); if (np == NULL) #endif { np = (char *) malloc (namelen + 1 + vallen); if (np == NULL) { #if defined USE_TSEARCH && !defined _LIBC freea (new_value); #endif __set_errno (ENOMEM); UNLOCK; return -1; } #ifdef USE_TSEARCH memcpy (np, new_value, namelen + 1 + vallen); #else memcpy (np, name, namelen); np[namelen] = '='; memcpy (&np[namelen + 1], value, vallen); #endif /* And remember the value. */ STORE_VALUE (np); } #if defined USE_TSEARCH && !defined _LIBC freea (new_value); #endif } *ep = np; } UNLOCK; return 0; } int setenv (const char *name, const char *value, int replace) { if (name == NULL || *name == '\0' || strchr (name, '=') != NULL) { __set_errno (EINVAL); return -1; } return __add_to_environ (name, value, NULL, replace); } /* The 'clearenv' was planned to be added to POSIX.1 but probably never made it. Nevertheless the POSIX.9 standard (POSIX bindings for Fortran 77) requires this function. */ int clearenv (void) { LOCK; if (__environ == last_environ && __environ != NULL) { /* We allocated this environment so we can free it. */ free (__environ); last_environ = NULL; } /* Clear the environment pointer removes the whole environment. */ __environ = NULL; UNLOCK; return 0; } #ifdef _LIBC static void free_mem (void) { /* Remove all traces. */ clearenv (); /* Now remove the search tree. */ __tdestroy (known_values, free); known_values = NULL; } text_set_element (__libc_subfreeres, free_mem); # undef setenv # undef clearenv weak_alias (__setenv, setenv) weak_alias (__clearenv, clearenv) #endif #endif /* _LIBC || !HAVE_SETENV */ /* The rest of this file is called into use when replacing an existing but buggy setenv. Known bugs include failure to diagnose invalid name, and consuming a leading '=' from value. */ #if HAVE_SETENV # undef setenv # if !HAVE_DECL_SETENV extern int setenv (const char *, const char *, int); # endif # define STREQ(a, b) (strcmp (a, b) == 0) int rpl_setenv (const char *name, const char *value, int replace) { int result; if (!name || !*name || strchr (name, '=')) { errno = EINVAL; return -1; } /* Call the real setenv even if replace is 0, in case implementation has underlying data to update, such as when environ changes. */ result = setenv (name, value, replace); if (result == 0 && replace && *value == '=') { char *tmp = getenv (name); if (!STREQ (tmp, value)) { int saved_errno; size_t len = strlen (value); tmp = malloca (len + 2); /* Since leading '=' is eaten, double it up. */ *tmp = '='; memcpy (tmp + 1, value, len + 1); result = setenv (name, tmp, replace); saved_errno = errno; freea (tmp); errno = saved_errno; } } return result; } #endif /* HAVE_SETENV */ gnuastro-0.2.33-8a3b/bootstrapped/tests/putenv.c0000644000175000017500000001176313004436755016471 00000000000000/* Copyright (C) 1991, 1994, 1997-1998, 2000, 2003-2016 Free Software Foundation, Inc. NOTE: The canonical source of this file is maintained with the GNU C Library. Bugs can be reported to bug-glibc@prep.ai.mit.edu. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include /* Include errno.h *after* sys/types.h to work around header problems on AIX 3.2.5. */ #include #ifndef __set_errno # define __set_errno(ev) ((errno) = (ev)) #endif #include #include #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # define WIN32_LEAN_AND_MEAN # include #endif #if _LIBC # if HAVE_GNU_LD # define environ __environ # else extern char **environ; # endif #endif #if _LIBC /* This lock protects against simultaneous modifications of 'environ'. */ # include __libc_lock_define_initialized (static, envlock) # define LOCK __libc_lock_lock (envlock) # define UNLOCK __libc_lock_unlock (envlock) #else # define LOCK # define UNLOCK #endif static int _unsetenv (const char *name) { size_t len; #if !HAVE_DECL__PUTENV char **ep; #endif if (name == NULL || *name == '\0' || strchr (name, '=') != NULL) { __set_errno (EINVAL); return -1; } len = strlen (name); #if HAVE_DECL__PUTENV { int putenv_result, putenv_errno; char *name_ = malloc (len + 2); memcpy (name_, name, len); name_[len] = '='; name_[len + 1] = 0; putenv_result = _putenv (name_); putenv_errno = errno; free (name_); __set_errno (putenv_errno); return putenv_result; } #else LOCK; ep = environ; while (*ep != NULL) if (!strncmp (*ep, name, len) && (*ep)[len] == '=') { /* Found it. Remove this pointer by moving later ones back. */ char **dp = ep; do dp[0] = dp[1]; while (*dp++); /* Continue the loop in case NAME appears again. */ } else ++ep; UNLOCK; return 0; #endif } /* Put STRING, which is of the form "NAME=VALUE", in the environment. If STRING contains no '=', then remove STRING from the environment. */ int putenv (char *string) { const char *name_end = strchr (string, '='); char **ep; if (name_end == NULL) { /* Remove the variable from the environment. */ return _unsetenv (string); } #if HAVE_DECL__PUTENV /* Rely on _putenv to allocate the new environment. If other parts of the application use _putenv, the !HAVE_DECL__PUTENV code would fight over who owns the environ vector, causing a crash. */ if (name_end[1]) return _putenv (string); else { /* _putenv ("NAME=") unsets NAME, so invoke _putenv ("NAME= ") to allocate the environ vector and then replace the new entry with "NAME=". */ int putenv_result, putenv_errno; char *name_x = malloc (name_end - string + sizeof "= "); if (!name_x) return -1; memcpy (name_x, string, name_end - string + 1); name_x[name_end - string + 1] = ' '; name_x[name_end - string + 2] = 0; putenv_result = _putenv (name_x); putenv_errno = errno; for (ep = environ; *ep; ep++) if (strcmp (*ep, name_x) == 0) { *ep = string; break; } # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ if (putenv_result == 0) { /* _putenv propagated "NAME= " into the subprocess environment; fix that by calling SetEnvironmentVariable directly. */ name_x[name_end - string] = 0; putenv_result = SetEnvironmentVariable (name_x, "") ? 0 : -1; putenv_errno = ENOMEM; /* ENOMEM is the only way to fail. */ } # endif free (name_x); __set_errno (putenv_errno); return putenv_result; } #else for (ep = environ; *ep; ep++) if (strncmp (*ep, string, name_end - string) == 0 && (*ep)[name_end - string] == '=') break; if (*ep) *ep = string; else { static char **last_environ = NULL; size_t size = ep - environ; char **new_environ = malloc ((size + 2) * sizeof *new_environ); if (! new_environ) return -1; new_environ[0] = string; memcpy (new_environ + 1, environ, (size + 1) * sizeof *new_environ); free (last_environ); last_environ = new_environ; environ = new_environ; } return 0; #endif } gnuastro-0.2.33-8a3b/bootstrapped/tests/open.c0000644000175000017500000001375513004436755016114 00000000000000/* Open a descriptor to a file. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ /* If the user's config.h happens to include , let it include only the system's here, so that orig_open doesn't recurse to rpl_open. */ #define __need_system_fcntl_h #include /* Get the original definition of open. It might be defined as a macro. */ #include #include #undef __need_system_fcntl_h static int orig_open (const char *filename, int flags, mode_t mode) { return open (filename, flags, mode); } /* Specification. */ /* Write "fcntl.h" here, not , otherwise OSF/1 5.1 DTK cc eliminates this include because of the preliminary #include above. */ #include "fcntl.h" #include #include #include #include #include #include #ifndef REPLACE_OPEN_DIRECTORY # define REPLACE_OPEN_DIRECTORY 0 #endif int open (const char *filename, int flags, ...) { mode_t mode; int fd; mode = 0; if (flags & O_CREAT) { va_list arg; va_start (arg, flags); /* We have to use PROMOTED_MODE_T instead of mode_t, otherwise GCC 4 creates crashing code when 'mode_t' is smaller than 'int'. */ mode = va_arg (arg, PROMOTED_MODE_T); va_end (arg); } #if GNULIB_defined_O_NONBLOCK /* The only known platform that lacks O_NONBLOCK is mingw, but it also lacks named pipes and Unix sockets, which are the only two file types that require non-blocking handling in open(). Therefore, it is safe to ignore O_NONBLOCK here. It is handy that mingw also lacks openat(), so that is also covered here. */ flags &= ~O_NONBLOCK; #endif #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ if (strcmp (filename, "/dev/null") == 0) filename = "NUL"; #endif #if OPEN_TRAILING_SLASH_BUG /* If the filename ends in a slash and one of O_CREAT, O_WRONLY, O_RDWR is specified, then fail. Rationale: POSIX says that "A pathname that contains at least one non-slash character and that ends with one or more trailing slashes shall be resolved as if a single dot character ( '.' ) were appended to the pathname." and "The special filename dot shall refer to the directory specified by its predecessor." If the named file already exists as a directory, then - if O_CREAT is specified, open() must fail because of the semantics of O_CREAT, - if O_WRONLY or O_RDWR is specified, open() must fail because POSIX says that it fails with errno = EISDIR in this case. If the named file does not exist or does not name a directory, then - if O_CREAT is specified, open() must fail since open() cannot create directories, - if O_WRONLY or O_RDWR is specified, open() must fail because the file does not contain a '.' directory. */ if (flags & (O_CREAT | O_WRONLY | O_RDWR)) { size_t len = strlen (filename); if (len > 0 && filename[len - 1] == '/') { errno = EISDIR; return -1; } } #endif fd = orig_open (filename, flags, mode); #if REPLACE_FCHDIR /* Implementing fchdir and fdopendir requires the ability to open a directory file descriptor. If open doesn't support that (as on mingw), we use a dummy file that behaves the same as directories on Linux (ie. always reports EOF on attempts to read()), and override fstat() in fchdir.c to hide the fact that we have a dummy. */ if (REPLACE_OPEN_DIRECTORY && fd < 0 && errno == EACCES && ((flags & O_ACCMODE) == O_RDONLY || (O_SEARCH != O_RDONLY && (flags & O_ACCMODE) == O_SEARCH))) { struct stat statbuf; if (stat (filename, &statbuf) == 0 && S_ISDIR (statbuf.st_mode)) { /* Maximum recursion depth of 1. */ fd = open ("/dev/null", flags, mode); if (0 <= fd) fd = _gl_register_fd (fd, filename); } else errno = EACCES; } #endif #if OPEN_TRAILING_SLASH_BUG /* If the filename ends in a slash and fd does not refer to a directory, then fail. Rationale: POSIX says that "A pathname that contains at least one non-slash character and that ends with one or more trailing slashes shall be resolved as if a single dot character ( '.' ) were appended to the pathname." and "The special filename dot shall refer to the directory specified by its predecessor." If the named file without the slash is not a directory, open() must fail with ENOTDIR. */ if (fd >= 0) { /* We know len is positive, since open did not fail with ENOENT. */ size_t len = strlen (filename); if (filename[len - 1] == '/') { struct stat statbuf; if (fstat (fd, &statbuf) >= 0 && !S_ISDIR (statbuf.st_mode)) { close (fd); errno = ENOTDIR; return -1; } } } #endif #if REPLACE_FCHDIR if (!REPLACE_OPEN_DIRECTORY && 0 <= fd) fd = _gl_register_fd (fd, filename); #endif return fd; } gnuastro-0.2.33-8a3b/bootstrapped/tests/lstat.c0000644000175000017500000000667413004436755016304 00000000000000/* Work around a bug of lstat on some systems Copyright (C) 1997-2006, 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* written by Jim Meyering */ /* If the user's config.h happens to include , let it include only the system's here, so that orig_lstat doesn't recurse to rpl_lstat. */ #define __need_system_sys_stat_h #include #if !HAVE_LSTAT /* On systems that lack symlinks, our replacement already defined lstat as stat, so there is nothing further to do other than avoid an empty file. */ typedef int dummy; #else /* HAVE_LSTAT */ /* Get the original definition of lstat. It might be defined as a macro. */ # include # include # undef __need_system_sys_stat_h static int orig_lstat (const char *filename, struct stat *buf) { return lstat (filename, buf); } /* Specification. */ /* Write "sys/stat.h" here, not , otherwise OSF/1 5.1 DTK cc eliminates this include because of the preliminary #include above. */ # include "sys/stat.h" # include # include /* lstat works differently on Linux and Solaris systems. POSIX (see "pathname resolution" in the glossary) requires that programs like 'ls' take into consideration the fact that FILE has a trailing slash when FILE is a symbolic link. On Linux and Solaris 10 systems, the lstat function already has the desired semantics (in treating 'lstat ("symlink/", sbuf)' just like 'lstat ("symlink/.", sbuf)', but on Solaris 9 and earlier it does not. If FILE has a trailing slash and specifies a symbolic link, then use stat() to get more info on the referent of FILE. If the referent is a non-directory, then set errno to ENOTDIR and return -1. Otherwise, return stat's result. */ int rpl_lstat (const char *file, struct stat *sbuf) { size_t len; int lstat_result = orig_lstat (file, sbuf); if (lstat_result != 0) return lstat_result; /* This replacement file can blindly check against '/' rather than using the ISSLASH macro, because all platforms with '\\' either lack symlinks (mingw) or have working lstat (cygwin) and thus do not compile this file. 0 len should have already been filtered out above, with a failure return of ENOENT. */ len = strlen (file); if (file[len - 1] != '/' || S_ISDIR (sbuf->st_mode)) return 0; /* At this point, a trailing slash is only permitted on symlink-to-dir; but it should have found information on the directory, not the symlink. Call stat() to get info about the link's referent. Our replacement stat guarantees valid results, even if the symlink is not pointing to a directory. */ if (!S_ISLNK (sbuf->st_mode)) { errno = ENOTDIR; return -1; } return stat (file, sbuf); } #endif /* HAVE_LSTAT */ gnuastro-0.2.33-8a3b/bootstrapped/tests/gettimeofday.c0000644000175000017500000000775113004436755017633 00000000000000/* Provide gettimeofday for systems that don't have it or for which it's broken. Copyright (C) 2001-2003, 2005-2007, 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* written by Jim Meyering */ #include /* Specification. */ #include #include #if HAVE_SYS_TIMEB_H # include #endif #if GETTIMEOFDAY_CLOBBERS_LOCALTIME || TZSET_CLOBBERS_LOCALTIME /* Work around the bug in some systems whereby gettimeofday clobbers the static buffer that localtime uses for its return value. The gettimeofday function from Mac OS X 10.0.4 (i.e., Darwin 1.3.7) has this problem. The tzset replacement is necessary for at least Solaris 2.5, 2.5.1, and 2.6. */ static struct tm tm_zero_buffer; static struct tm *localtime_buffer_addr = &tm_zero_buffer; # undef localtime extern struct tm *localtime (time_t const *); # undef gmtime extern struct tm *gmtime (time_t const *); /* This is a wrapper for localtime. It is used only on systems for which gettimeofday clobbers the static buffer used for localtime's result. On the first call, record the address of the static buffer that localtime uses for its result. */ struct tm * rpl_localtime (time_t const *timep) { struct tm *tm = localtime (timep); if (localtime_buffer_addr == &tm_zero_buffer) localtime_buffer_addr = tm; return tm; } /* Same as above, since gmtime and localtime use the same buffer. */ struct tm * rpl_gmtime (time_t const *timep) { struct tm *tm = gmtime (timep); if (localtime_buffer_addr == &tm_zero_buffer) localtime_buffer_addr = tm; return tm; } #endif /* GETTIMEOFDAY_CLOBBERS_LOCALTIME || TZSET_CLOBBERS_LOCALTIME */ #if TZSET_CLOBBERS_LOCALTIME # undef tzset extern void tzset (void); /* This is a wrapper for tzset, for systems on which tzset may clobber the static buffer used for localtime's result. */ void rpl_tzset (void) { /* Save and restore the contents of the buffer used for localtime's result around the call to tzset. */ struct tm save = *localtime_buffer_addr; tzset (); *localtime_buffer_addr = save; } #endif /* This is a wrapper for gettimeofday. It is used only on systems that lack this function, or whose implementation of this function causes problems. */ int gettimeofday (struct timeval *restrict tv, void *restrict tz) { #undef gettimeofday #if HAVE_GETTIMEOFDAY # if GETTIMEOFDAY_CLOBBERS_LOCALTIME /* Save and restore the contents of the buffer used for localtime's result around the call to gettimeofday. */ struct tm save = *localtime_buffer_addr; # endif # if defined timeval /* 'struct timeval' overridden by gnulib? */ # undef timeval struct timeval otv; int result = gettimeofday (&otv, (struct timezone *) tz); if (result == 0) { tv->tv_sec = otv.tv_sec; tv->tv_usec = otv.tv_usec; } # else int result = gettimeofday (tv, (struct timezone *) tz); # endif # if GETTIMEOFDAY_CLOBBERS_LOCALTIME *localtime_buffer_addr = save; # endif return result; #else # if HAVE__FTIME struct _timeb timebuf; _ftime (&timebuf); tv->tv_sec = timebuf.time; tv->tv_usec = timebuf.millitm * 1000; # else # if !defined OK_TO_USE_1S_CLOCK # error "Only 1-second nominal clock resolution found. Is that intended?" \ "If so, compile with the -DOK_TO_USE_1S_CLOCK option." # endif tv->tv_sec = time (NULL); tv->tv_usec = 0; # endif return 0; #endif } gnuastro-0.2.33-8a3b/bootstrapped/tests/getpagesize.c0000644000175000017500000000227413004436755017454 00000000000000/* getpagesize emulation for systems where it cannot be done in a C macro. Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible and Martin Lambers. */ #include /* Specification. */ #include /* This implementation is only for native Windows systems. */ #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # define WIN32_LEAN_AND_MEAN # include int getpagesize (void) { SYSTEM_INFO system_info; GetSystemInfo (&system_info); return system_info.dwPageSize; } #endif gnuastro-0.2.33-8a3b/bootstrapped/tests/getdtablesize.c0000644000175000017500000000643713004436755020000 00000000000000/* getdtablesize() function for platforms that don't have it. Copyright (C) 2008-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2008. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # include # include "msvc-inval.h" # if HAVE_MSVC_INVALID_PARAMETER_HANDLER static int _setmaxstdio_nothrow (int newmax) { int result; TRY_MSVC_INVAL { result = _setmaxstdio (newmax); } CATCH_MSVC_INVAL { result = -1; } DONE_MSVC_INVAL; return result; } # define _setmaxstdio _setmaxstdio_nothrow # endif /* Cache for the previous getdtablesize () result. Safe to cache because Windows also lacks setrlimit. */ static int dtablesize; int getdtablesize (void) { if (dtablesize == 0) { /* We are looking for the number N such that the valid file descriptors are 0..N-1. It can be obtained through a loop as follows: { int fd; for (fd = 3; fd < 65536; fd++) if (dup2 (0, fd) == -1) break; return fd; } On Windows XP, the result is 2048. The drawback of this loop is that it allocates memory for a libc internal array that is never freed. The number N can also be obtained as the upper bound for _getmaxstdio (). _getmaxstdio () returns the maximum number of open FILE objects. The sanity check in _setmaxstdio reveals the maximum number of file descriptors. This too allocates memory, but it is freed when we call _setmaxstdio with the original value. */ int orig_max_stdio = _getmaxstdio (); unsigned int bound; for (bound = 0x10000; _setmaxstdio (bound) < 0; bound = bound / 2) ; _setmaxstdio (orig_max_stdio); dtablesize = bound; } return dtablesize; } #else # include # include # ifndef RLIM_SAVED_CUR # define RLIM_SAVED_CUR RLIM_INFINITY # endif # ifndef RLIM_SAVED_MAX # define RLIM_SAVED_MAX RLIM_INFINITY # endif # ifdef __CYGWIN__ /* Cygwin 1.7.25 auto-increases the RLIMIT_NOFILE soft limit until it hits the compile-time constant hard limit of 3200. We might as well just report the hard limit. */ # define rlim_cur rlim_max # endif int getdtablesize (void) { struct rlimit lim; if (getrlimit (RLIMIT_NOFILE, &lim) == 0 && 0 <= lim.rlim_cur && lim.rlim_cur <= INT_MAX && lim.rlim_cur != RLIM_INFINITY && lim.rlim_cur != RLIM_SAVED_CUR && lim.rlim_cur != RLIM_SAVED_MAX) return lim.rlim_cur; return INT_MAX; } #endif gnuastro-0.2.33-8a3b/bootstrapped/tests/getcwd-lgpl.c0000644000175000017500000000606613004436755017361 00000000000000/* Copyright (C) 2011-2016 Free Software Foundation, Inc. This file is part of gnulib. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification */ #include #include #include #include #if GNULIB_GETCWD /* Favor GPL getcwd.c if both getcwd and getcwd-lgpl modules are in use. */ typedef int dummy; #else /* Get the name of the current working directory, and put it in SIZE bytes of BUF. Returns NULL if the directory couldn't be determined (perhaps because the absolute name was longer than PATH_MAX, or because of missing read/search permissions on parent directories) or SIZE was too small. If successful, returns BUF. If BUF is NULL, an array is allocated with 'malloc'; the array is SIZE bytes long, unless SIZE == 0, in which case it is as big as necessary. */ # undef getcwd char * rpl_getcwd (char *buf, size_t size) { char *ptr; char *result; /* Handle single size operations. */ if (buf) { if (!size) { errno = EINVAL; return NULL; } return getcwd (buf, size); } if (size) { buf = malloc (size); if (!buf) { errno = ENOMEM; return NULL; } result = getcwd (buf, size); if (!result) { int saved_errno = errno; free (buf); errno = saved_errno; } return result; } /* Flexible sizing requested. Avoid over-allocation for the common case of a name that fits within a 4k page, minus some space for local variables, to be sure we don't skip over a guard page. */ { char tmp[4032]; size = sizeof tmp; ptr = getcwd (tmp, size); if (ptr) { result = strdup (ptr); if (!result) errno = ENOMEM; return result; } if (errno != ERANGE) return NULL; } /* My what a large directory name we have. */ do { size <<= 1; ptr = realloc (buf, size); if (ptr == NULL) { free (buf); errno = ENOMEM; return NULL; } buf = ptr; result = getcwd (buf, size); } while (!result && errno == ERANGE); if (!result) { int saved_errno = errno; free (buf); errno = saved_errno; } else { /* Trim to fit, if possible. */ result = realloc (buf, strlen (buf) + 1); if (!result) result = buf; } return result; } #endif gnuastro-0.2.33-8a3b/bootstrapped/tests/fstat.c0000644000175000017500000000460513004436755016266 00000000000000/* fstat() replacement. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* If the user's config.h happens to include , let it include only the system's here, so that orig_fstat doesn't recurse to rpl_fstat. */ #define __need_system_sys_stat_h #include /* Get the original definition of fstat. It might be defined as a macro. */ #include #include #if _GL_WINDOWS_64_BIT_ST_SIZE # undef stat /* avoid warning on mingw64 with _FILE_OFFSET_BITS=64 */ # define stat _stati64 # undef fstat /* avoid warning on mingw64 with _FILE_OFFSET_BITS=64 */ # define fstat _fstati64 #endif #undef __need_system_sys_stat_h static int orig_fstat (int fd, struct stat *buf) { return fstat (fd, buf); } /* Specification. */ /* Write "sys/stat.h" here, not , otherwise OSF/1 5.1 DTK cc eliminates this include because of the preliminary #include above. */ #include "sys/stat.h" #include #include #if HAVE_MSVC_INVALID_PARAMETER_HANDLER # include "msvc-inval.h" #endif #if HAVE_MSVC_INVALID_PARAMETER_HANDLER static int fstat_nothrow (int fd, struct stat *buf) { int result; TRY_MSVC_INVAL { result = orig_fstat (fd, buf); } CATCH_MSVC_INVAL { result = -1; errno = EBADF; } DONE_MSVC_INVAL; return result; } #else # define fstat_nothrow orig_fstat #endif int rpl_fstat (int fd, struct stat *buf) { #if REPLACE_FCHDIR && REPLACE_OPEN_DIRECTORY /* Handle the case when rpl_open() used a dummy file descriptor to work around an open() that can't normally visit directories. */ const char *name = _gl_directory_name (fd); if (name != NULL) return stat (name, buf); #endif return fstat_nothrow (fd, buf); } gnuastro-0.2.33-8a3b/bootstrapped/tests/fdopen.c0000644000175000017500000000272713004436755016423 00000000000000/* Open a stream with a given file descriptor. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #if HAVE_MSVC_INVALID_PARAMETER_HANDLER # include "msvc-inval.h" #endif #undef fdopen #if HAVE_MSVC_INVALID_PARAMETER_HANDLER static FILE * fdopen_nothrow (int fd, const char *mode) { FILE *result; TRY_MSVC_INVAL { result = fdopen (fd, mode); } CATCH_MSVC_INVAL { result = NULL; } DONE_MSVC_INVAL; return result; } #else # define fdopen_nothrow fdopen #endif FILE * rpl_fdopen (int fd, const char *mode) { int saved_errno = errno; FILE *fp; errno = 0; fp = fdopen_nothrow (fd, mode); if (fp == NULL) { if (errno == 0) errno = EBADF; } else errno = saved_errno; return fp; } gnuastro-0.2.33-8a3b/bootstrapped/tests/dup2.c0000644000175000017500000001107513004436755016016 00000000000000/* Duplicate an open file descriptor to a specified file descriptor. Copyright (C) 1999, 2004-2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* written by Paul Eggert */ #include /* Specification. */ #include #include #include #if HAVE_DUP2 # undef dup2 # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Get declarations of the native Windows API functions. */ # define WIN32_LEAN_AND_MEAN # include # include "msvc-inval.h" /* Get _get_osfhandle. */ # include "msvc-nothrow.h" static int ms_windows_dup2 (int fd, int desired_fd) { int result; /* If fd is closed, mingw hangs on dup2 (fd, fd). If fd is open, dup2 (fd, fd) returns 0, but all further attempts to use fd in future dup2 calls will hang. */ if (fd == desired_fd) { if ((HANDLE) _get_osfhandle (fd) == INVALID_HANDLE_VALUE) { errno = EBADF; return -1; } return fd; } /* Wine 1.0.1 return 0 when desired_fd is negative but not -1: http://bugs.winehq.org/show_bug.cgi?id=21289 */ if (desired_fd < 0) { errno = EBADF; return -1; } TRY_MSVC_INVAL { result = dup2 (fd, desired_fd); } CATCH_MSVC_INVAL { errno = EBADF; result = -1; } DONE_MSVC_INVAL; if (result == 0) result = desired_fd; return result; } # define dup2 ms_windows_dup2 # elif defined __KLIBC__ # include static int klibc_dup2dirfd (int fd, int desired_fd) { int tempfd; int dupfd; tempfd = open ("NUL", O_RDONLY); if (tempfd == -1) return -1; if (tempfd == desired_fd) { close (tempfd); char path[_MAX_PATH]; if (__libc_Back_ioFHToPath (fd, path, sizeof (path))) return -1; return open(path, O_RDONLY); } dupfd = klibc_dup2dirfd (fd, desired_fd); close (tempfd); return dupfd; } static int klibc_dup2 (int fd, int desired_fd) { int dupfd; struct stat sbuf; dupfd = dup2 (fd, desired_fd); if (dupfd == -1 && errno == ENOTSUP \ && !fstat (fd, &sbuf) && S_ISDIR (sbuf.st_mode)) { close (desired_fd); return klibc_dup2dirfd (fd, desired_fd); } return dupfd; } # define dup2 klibc_dup2 # endif int rpl_dup2 (int fd, int desired_fd) { int result; # ifdef F_GETFL /* On Linux kernels 2.6.26-2.6.29, dup2 (fd, fd) returns -EBADF. On Cygwin 1.5.x, dup2 (1, 1) returns 0. On Cygwin 1.7.17, dup2 (1, -1) dumps core. On Cygwin 1.7.25, dup2 (1, 256) can dump core. On Haiku, dup2 (fd, fd) mistakenly clears FD_CLOEXEC. */ # if HAVE_SETDTABLESIZE setdtablesize (desired_fd + 1); # endif if (desired_fd < 0) fd = desired_fd; if (fd == desired_fd) return fcntl (fd, F_GETFL) == -1 ? -1 : fd; # endif result = dup2 (fd, desired_fd); /* Correct an errno value on FreeBSD 6.1 and Cygwin 1.5.x. */ if (result == -1 && errno == EMFILE) errno = EBADF; # if REPLACE_FCHDIR if (fd != desired_fd && result != -1) result = _gl_register_dup (fd, result); # endif return result; } #else /* !HAVE_DUP2 */ /* On older platforms, dup2 did not exist. */ # ifndef F_DUPFD static int dupfd (int fd, int desired_fd) { int duplicated_fd = dup (fd); if (duplicated_fd < 0 || duplicated_fd == desired_fd) return duplicated_fd; else { int r = dupfd (fd, desired_fd); int e = errno; close (duplicated_fd); errno = e; return r; } } # endif int dup2 (int fd, int desired_fd) { int result = fcntl (fd, F_GETFL) < 0 ? -1 : fd; if (result == -1 || fd == desired_fd) return result; close (desired_fd); # ifdef F_DUPFD result = fcntl (fd, F_DUPFD, desired_fd); # if REPLACE_FCHDIR if (0 <= result) result = _gl_register_dup (fd, result); # endif # else result = dupfd (fd, desired_fd); # endif if (result == -1 && (errno == EMFILE || errno == EINVAL)) errno = EBADF; return result; } #endif /* !HAVE_DUP2 */ gnuastro-0.2.33-8a3b/bootstrapped/tests/close.c0000644000175000017500000000270713004436755016253 00000000000000/* close replacement. Copyright (C) 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include "fd-hook.h" #include "msvc-inval.h" #undef close #if HAVE_MSVC_INVALID_PARAMETER_HANDLER static int close_nothrow (int fd) { int result; TRY_MSVC_INVAL { result = close (fd); } CATCH_MSVC_INVAL { result = -1; errno = EBADF; } DONE_MSVC_INVAL; return result; } #else # define close_nothrow close #endif /* Override close() to call into other gnulib modules. */ int rpl_close (int fd) { #if WINDOWS_SOCKETS int retval = execute_all_close_hooks (close_nothrow, fd); #else int retval = close_nothrow (fd); #endif #if REPLACE_FCHDIR if (retval >= 0) _gl_unregister_fd (fd); #endif return retval; } gnuastro-0.2.33-8a3b/bootstrapped/tests/malloca.c0000644000175000017500000001157613004436755016562 00000000000000/* Safe automatic memory allocation. Copyright (C) 2003, 2006-2007, 2009-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2003. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #define _GL_USE_STDLIB_ALLOC 1 #include /* Specification. */ #include "malloca.h" #include #include "verify.h" /* The speed critical point in this file is freea() applied to an alloca() result: it must be fast, to match the speed of alloca(). The speed of mmalloca() and freea() in the other case are not critical, because they are only invoked for big memory sizes. */ #if HAVE_ALLOCA /* Store the mmalloca() results in a hash table. This is needed to reliably distinguish a mmalloca() result and an alloca() result. Although it is possible that the same pointer is returned by alloca() and by mmalloca() at different times in the same application, it does not lead to a bug in freea(), because: - Before a pointer returned by alloca() can point into malloc()ed memory, the function must return, and once this has happened the programmer must not call freea() on it anyway. - Before a pointer returned by mmalloca() can point into the stack, it must be freed. The only function that can free it is freea(), and when freea() frees it, it also removes it from the hash table. */ #define MAGIC_NUMBER 0x1415fb4a #define MAGIC_SIZE sizeof (int) /* This is how the header info would look like without any alignment considerations. */ struct preliminary_header { void *next; int magic; }; /* But the header's size must be a multiple of sa_alignment_max. */ #define HEADER_SIZE \ (((sizeof (struct preliminary_header) + sa_alignment_max - 1) / sa_alignment_max) * sa_alignment_max) union header { void *next; struct { char room[HEADER_SIZE - MAGIC_SIZE]; int word; } magic; }; verify (HEADER_SIZE == sizeof (union header)); /* We make the hash table quite big, so that during lookups the probability of empty hash buckets is quite high. There is no need to make the hash table resizable, because when the hash table gets filled so much that the lookup becomes slow, it means that the application has memory leaks. */ #define HASH_TABLE_SIZE 257 static void * mmalloca_results[HASH_TABLE_SIZE]; #endif void * mmalloca (size_t n) { #if HAVE_ALLOCA /* Allocate one more word, that serves as an indicator for malloc()ed memory, so that freea() of an alloca() result is fast. */ size_t nplus = n + HEADER_SIZE; if (nplus >= n) { void *p = malloc (nplus); if (p != NULL) { size_t slot; union header *h = p; p = h + 1; /* Put a magic number into the indicator word. */ h->magic.word = MAGIC_NUMBER; /* Enter p into the hash table. */ slot = (uintptr_t) p % HASH_TABLE_SIZE; h->next = mmalloca_results[slot]; mmalloca_results[slot] = p; return p; } } /* Out of memory. */ return NULL; #else # if !MALLOC_0_IS_NONNULL if (n == 0) n = 1; # endif return malloc (n); #endif } #if HAVE_ALLOCA void freea (void *p) { /* mmalloca() may have returned NULL. */ if (p != NULL) { /* Attempt to quickly distinguish the mmalloca() result - which has a magic indicator word - and the alloca() result - which has an uninitialized indicator word. It is for this test that sa_increment additional bytes are allocated in the alloca() case. */ if (((int *) p)[-1] == MAGIC_NUMBER) { /* Looks like a mmalloca() result. To see whether it really is one, perform a lookup in the hash table. */ size_t slot = (uintptr_t) p % HASH_TABLE_SIZE; void **chain = &mmalloca_results[slot]; for (; *chain != NULL;) { union header *h = p; if (*chain == p) { /* Found it. Remove it from the hash table and free it. */ union header *p_begin = h - 1; *chain = p_begin->next; free (p_begin); return; } h = *chain; chain = &h[-1].next; } } /* At this point, we know it was not a mmalloca() result. */ } } #endif gnuastro-0.2.33-8a3b/bootstrapped/tests/localename.c0000644000175000017500000025017113004436755017246 00000000000000/* Determine name of the currently selected locale. Copyright (C) 1995-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Ulrich Drepper , 1995. */ /* Native Windows code written by Tor Lillqvist . */ /* Mac OS X code written by Bruno Haible . */ #include /* Specification. */ #ifdef IN_LIBINTL # include "gettextP.h" #else # include "localename.h" #endif #include #include #include #include #include #include "flexmember.h" #if HAVE_USELOCALE /* Mac OS X 10.5 defines the locale_t type in . */ # if defined __APPLE__ && defined __MACH__ # include # endif # if __GLIBC__ >= 2 && !defined __UCLIBC__ # include # endif # if !defined IN_LIBINTL # include "glthread/lock.h" # endif # if defined __sun && HAVE_GETLOCALENAME_L /* Solaris >= 12. */ extern char * getlocalename_l(int, locale_t); # endif #endif #if HAVE_CFLOCALECOPYCURRENT || HAVE_CFPREFERENCESCOPYAPPVALUE # include # if HAVE_CFLOCALECOPYCURRENT # include # elif HAVE_CFPREFERENCESCOPYAPPVALUE # include # endif #endif #if defined _WIN32 || defined __WIN32__ # define WINDOWS_NATIVE # if !defined IN_LIBINTL # include "glthread/lock.h" # endif #endif #if defined WINDOWS_NATIVE || defined __CYGWIN__ /* Native Windows or Cygwin */ # define WIN32_LEAN_AND_MEAN # include # include /* List of language codes, sorted by value: 0x01 LANG_ARABIC 0x02 LANG_BULGARIAN 0x03 LANG_CATALAN 0x04 LANG_CHINESE 0x05 LANG_CZECH 0x06 LANG_DANISH 0x07 LANG_GERMAN 0x08 LANG_GREEK 0x09 LANG_ENGLISH 0x0a LANG_SPANISH 0x0b LANG_FINNISH 0x0c LANG_FRENCH 0x0d LANG_HEBREW 0x0e LANG_HUNGARIAN 0x0f LANG_ICELANDIC 0x10 LANG_ITALIAN 0x11 LANG_JAPANESE 0x12 LANG_KOREAN 0x13 LANG_DUTCH 0x14 LANG_NORWEGIAN 0x15 LANG_POLISH 0x16 LANG_PORTUGUESE 0x17 LANG_ROMANSH 0x18 LANG_ROMANIAN 0x19 LANG_RUSSIAN 0x1a LANG_CROATIAN == LANG_SERBIAN 0x1b LANG_SLOVAK 0x1c LANG_ALBANIAN 0x1d LANG_SWEDISH 0x1e LANG_THAI 0x1f LANG_TURKISH 0x20 LANG_URDU 0x21 LANG_INDONESIAN 0x22 LANG_UKRAINIAN 0x23 LANG_BELARUSIAN 0x24 LANG_SLOVENIAN 0x25 LANG_ESTONIAN 0x26 LANG_LATVIAN 0x27 LANG_LITHUANIAN 0x28 LANG_TAJIK 0x29 LANG_FARSI 0x2a LANG_VIETNAMESE 0x2b LANG_ARMENIAN 0x2c LANG_AZERI 0x2d LANG_BASQUE 0x2e LANG_SORBIAN 0x2f LANG_MACEDONIAN 0x30 LANG_SUTU 0x31 LANG_TSONGA 0x32 LANG_TSWANA 0x33 LANG_VENDA 0x34 LANG_XHOSA 0x35 LANG_ZULU 0x36 LANG_AFRIKAANS 0x37 LANG_GEORGIAN 0x38 LANG_FAEROESE 0x39 LANG_HINDI 0x3a LANG_MALTESE 0x3b LANG_SAMI 0x3c LANG_GAELIC 0x3d LANG_YIDDISH 0x3e LANG_MALAY 0x3f LANG_KAZAK 0x40 LANG_KYRGYZ 0x41 LANG_SWAHILI 0x42 LANG_TURKMEN 0x43 LANG_UZBEK 0x44 LANG_TATAR 0x45 LANG_BENGALI 0x46 LANG_PUNJABI 0x47 LANG_GUJARATI 0x48 LANG_ORIYA 0x49 LANG_TAMIL 0x4a LANG_TELUGU 0x4b LANG_KANNADA 0x4c LANG_MALAYALAM 0x4d LANG_ASSAMESE 0x4e LANG_MARATHI 0x4f LANG_SANSKRIT 0x50 LANG_MONGOLIAN 0x51 LANG_TIBETAN 0x52 LANG_WELSH 0x53 LANG_CAMBODIAN 0x54 LANG_LAO 0x55 LANG_BURMESE 0x56 LANG_GALICIAN 0x57 LANG_KONKANI 0x58 LANG_MANIPURI 0x59 LANG_SINDHI 0x5a LANG_SYRIAC 0x5b LANG_SINHALESE 0x5c LANG_CHEROKEE 0x5d LANG_INUKTITUT 0x5e LANG_AMHARIC 0x5f LANG_TAMAZIGHT 0x60 LANG_KASHMIRI 0x61 LANG_NEPALI 0x62 LANG_FRISIAN 0x63 LANG_PASHTO 0x64 LANG_TAGALOG 0x65 LANG_DIVEHI 0x66 LANG_EDO 0x67 LANG_FULFULDE 0x68 LANG_HAUSA 0x69 LANG_IBIBIO 0x6a LANG_YORUBA 0x6d LANG_BASHKIR 0x6e LANG_LUXEMBOURGISH 0x6f LANG_GREENLANDIC 0x70 LANG_IGBO 0x71 LANG_KANURI 0x72 LANG_OROMO 0x73 LANG_TIGRINYA 0x74 LANG_GUARANI 0x75 LANG_HAWAIIAN 0x76 LANG_LATIN 0x77 LANG_SOMALI 0x78 LANG_YI 0x79 LANG_PAPIAMENTU 0x7a LANG_MAPUDUNGUN 0x7c LANG_MOHAWK 0x7e LANG_BRETON 0x82 LANG_OCCITAN 0x83 LANG_CORSICAN 0x84 LANG_ALSATIAN 0x85 LANG_YAKUT 0x86 LANG_KICHE 0x87 LANG_KINYARWANDA 0x88 LANG_WOLOF 0x8c LANG_DARI 0x91 LANG_SCOTTISH_GAELIC */ /* Mingw headers don't have latest language and sublanguage codes. */ # ifndef LANG_AFRIKAANS # define LANG_AFRIKAANS 0x36 # endif # ifndef LANG_ALBANIAN # define LANG_ALBANIAN 0x1c # endif # ifndef LANG_ALSATIAN # define LANG_ALSATIAN 0x84 # endif # ifndef LANG_AMHARIC # define LANG_AMHARIC 0x5e # endif # ifndef LANG_ARABIC # define LANG_ARABIC 0x01 # endif # ifndef LANG_ARMENIAN # define LANG_ARMENIAN 0x2b # endif # ifndef LANG_ASSAMESE # define LANG_ASSAMESE 0x4d # endif # ifndef LANG_AZERI # define LANG_AZERI 0x2c # endif # ifndef LANG_BASHKIR # define LANG_BASHKIR 0x6d # endif # ifndef LANG_BASQUE # define LANG_BASQUE 0x2d # endif # ifndef LANG_BELARUSIAN # define LANG_BELARUSIAN 0x23 # endif # ifndef LANG_BENGALI # define LANG_BENGALI 0x45 # endif # ifndef LANG_BRETON # define LANG_BRETON 0x7e # endif # ifndef LANG_BURMESE # define LANG_BURMESE 0x55 # endif # ifndef LANG_CAMBODIAN # define LANG_CAMBODIAN 0x53 # endif # ifndef LANG_CATALAN # define LANG_CATALAN 0x03 # endif # ifndef LANG_CHEROKEE # define LANG_CHEROKEE 0x5c # endif # ifndef LANG_CORSICAN # define LANG_CORSICAN 0x83 # endif # ifndef LANG_DARI # define LANG_DARI 0x8c # endif # ifndef LANG_DIVEHI # define LANG_DIVEHI 0x65 # endif # ifndef LANG_EDO # define LANG_EDO 0x66 # endif # ifndef LANG_ESTONIAN # define LANG_ESTONIAN 0x25 # endif # ifndef LANG_FAEROESE # define LANG_FAEROESE 0x38 # endif # ifndef LANG_FARSI # define LANG_FARSI 0x29 # endif # ifndef LANG_FRISIAN # define LANG_FRISIAN 0x62 # endif # ifndef LANG_FULFULDE # define LANG_FULFULDE 0x67 # endif # ifndef LANG_GAELIC # define LANG_GAELIC 0x3c # endif # ifndef LANG_GALICIAN # define LANG_GALICIAN 0x56 # endif # ifndef LANG_GEORGIAN # define LANG_GEORGIAN 0x37 # endif # ifndef LANG_GREENLANDIC # define LANG_GREENLANDIC 0x6f # endif # ifndef LANG_GUARANI # define LANG_GUARANI 0x74 # endif # ifndef LANG_GUJARATI # define LANG_GUJARATI 0x47 # endif # ifndef LANG_HAUSA # define LANG_HAUSA 0x68 # endif # ifndef LANG_HAWAIIAN # define LANG_HAWAIIAN 0x75 # endif # ifndef LANG_HEBREW # define LANG_HEBREW 0x0d # endif # ifndef LANG_HINDI # define LANG_HINDI 0x39 # endif # ifndef LANG_IBIBIO # define LANG_IBIBIO 0x69 # endif # ifndef LANG_IGBO # define LANG_IGBO 0x70 # endif # ifndef LANG_INDONESIAN # define LANG_INDONESIAN 0x21 # endif # ifndef LANG_INUKTITUT # define LANG_INUKTITUT 0x5d # endif # ifndef LANG_KANNADA # define LANG_KANNADA 0x4b # endif # ifndef LANG_KANURI # define LANG_KANURI 0x71 # endif # ifndef LANG_KASHMIRI # define LANG_KASHMIRI 0x60 # endif # ifndef LANG_KAZAK # define LANG_KAZAK 0x3f # endif # ifndef LANG_KICHE # define LANG_KICHE 0x86 # endif # ifndef LANG_KINYARWANDA # define LANG_KINYARWANDA 0x87 # endif # ifndef LANG_KONKANI # define LANG_KONKANI 0x57 # endif # ifndef LANG_KYRGYZ # define LANG_KYRGYZ 0x40 # endif # ifndef LANG_LAO # define LANG_LAO 0x54 # endif # ifndef LANG_LATIN # define LANG_LATIN 0x76 # endif # ifndef LANG_LATVIAN # define LANG_LATVIAN 0x26 # endif # ifndef LANG_LITHUANIAN # define LANG_LITHUANIAN 0x27 # endif # ifndef LANG_LUXEMBOURGISH # define LANG_LUXEMBOURGISH 0x6e # endif # ifndef LANG_MACEDONIAN # define LANG_MACEDONIAN 0x2f # endif # ifndef LANG_MALAY # define LANG_MALAY 0x3e # endif # ifndef LANG_MALAYALAM # define LANG_MALAYALAM 0x4c # endif # ifndef LANG_MALTESE # define LANG_MALTESE 0x3a # endif # ifndef LANG_MANIPURI # define LANG_MANIPURI 0x58 # endif # ifndef LANG_MAORI # define LANG_MAORI 0x81 # endif # ifndef LANG_MAPUDUNGUN # define LANG_MAPUDUNGUN 0x7a # endif # ifndef LANG_MARATHI # define LANG_MARATHI 0x4e # endif # ifndef LANG_MOHAWK # define LANG_MOHAWK 0x7c # endif # ifndef LANG_MONGOLIAN # define LANG_MONGOLIAN 0x50 # endif # ifndef LANG_NEPALI # define LANG_NEPALI 0x61 # endif # ifndef LANG_OCCITAN # define LANG_OCCITAN 0x82 # endif # ifndef LANG_ORIYA # define LANG_ORIYA 0x48 # endif # ifndef LANG_OROMO # define LANG_OROMO 0x72 # endif # ifndef LANG_PAPIAMENTU # define LANG_PAPIAMENTU 0x79 # endif # ifndef LANG_PASHTO # define LANG_PASHTO 0x63 # endif # ifndef LANG_PUNJABI # define LANG_PUNJABI 0x46 # endif # ifndef LANG_QUECHUA # define LANG_QUECHUA 0x6b # endif # ifndef LANG_ROMANSH # define LANG_ROMANSH 0x17 # endif # ifndef LANG_SAMI # define LANG_SAMI 0x3b # endif # ifndef LANG_SANSKRIT # define LANG_SANSKRIT 0x4f # endif # ifndef LANG_SCOTTISH_GAELIC # define LANG_SCOTTISH_GAELIC 0x91 # endif # ifndef LANG_SERBIAN # define LANG_SERBIAN 0x1a # endif # ifndef LANG_SINDHI # define LANG_SINDHI 0x59 # endif # ifndef LANG_SINHALESE # define LANG_SINHALESE 0x5b # endif # ifndef LANG_SLOVAK # define LANG_SLOVAK 0x1b # endif # ifndef LANG_SOMALI # define LANG_SOMALI 0x77 # endif # ifndef LANG_SORBIAN # define LANG_SORBIAN 0x2e # endif # ifndef LANG_SOTHO # define LANG_SOTHO 0x6c # endif # ifndef LANG_SUTU # define LANG_SUTU 0x30 # endif # ifndef LANG_SWAHILI # define LANG_SWAHILI 0x41 # endif # ifndef LANG_SYRIAC # define LANG_SYRIAC 0x5a # endif # ifndef LANG_TAGALOG # define LANG_TAGALOG 0x64 # endif # ifndef LANG_TAJIK # define LANG_TAJIK 0x28 # endif # ifndef LANG_TAMAZIGHT # define LANG_TAMAZIGHT 0x5f # endif # ifndef LANG_TAMIL # define LANG_TAMIL 0x49 # endif # ifndef LANG_TATAR # define LANG_TATAR 0x44 # endif # ifndef LANG_TELUGU # define LANG_TELUGU 0x4a # endif # ifndef LANG_THAI # define LANG_THAI 0x1e # endif # ifndef LANG_TIBETAN # define LANG_TIBETAN 0x51 # endif # ifndef LANG_TIGRINYA # define LANG_TIGRINYA 0x73 # endif # ifndef LANG_TSONGA # define LANG_TSONGA 0x31 # endif # ifndef LANG_TSWANA # define LANG_TSWANA 0x32 # endif # ifndef LANG_TURKMEN # define LANG_TURKMEN 0x42 # endif # ifndef LANG_UIGHUR # define LANG_UIGHUR 0x80 # endif # ifndef LANG_UKRAINIAN # define LANG_UKRAINIAN 0x22 # endif # ifndef LANG_URDU # define LANG_URDU 0x20 # endif # ifndef LANG_UZBEK # define LANG_UZBEK 0x43 # endif # ifndef LANG_VENDA # define LANG_VENDA 0x33 # endif # ifndef LANG_VIETNAMESE # define LANG_VIETNAMESE 0x2a # endif # ifndef LANG_WELSH # define LANG_WELSH 0x52 # endif # ifndef LANG_WOLOF # define LANG_WOLOF 0x88 # endif # ifndef LANG_XHOSA # define LANG_XHOSA 0x34 # endif # ifndef LANG_YAKUT # define LANG_YAKUT 0x85 # endif # ifndef LANG_YI # define LANG_YI 0x78 # endif # ifndef LANG_YIDDISH # define LANG_YIDDISH 0x3d # endif # ifndef LANG_YORUBA # define LANG_YORUBA 0x6a # endif # ifndef LANG_ZULU # define LANG_ZULU 0x35 # endif # ifndef SUBLANG_AFRIKAANS_SOUTH_AFRICA # define SUBLANG_AFRIKAANS_SOUTH_AFRICA 0x01 # endif # ifndef SUBLANG_ALBANIAN_ALBANIA # define SUBLANG_ALBANIAN_ALBANIA 0x01 # endif # ifndef SUBLANG_ALSATIAN_FRANCE # define SUBLANG_ALSATIAN_FRANCE 0x01 # endif # ifndef SUBLANG_AMHARIC_ETHIOPIA # define SUBLANG_AMHARIC_ETHIOPIA 0x01 # endif # ifndef SUBLANG_ARABIC_SAUDI_ARABIA # define SUBLANG_ARABIC_SAUDI_ARABIA 0x01 # endif # ifndef SUBLANG_ARABIC_IRAQ # define SUBLANG_ARABIC_IRAQ 0x02 # endif # ifndef SUBLANG_ARABIC_EGYPT # define SUBLANG_ARABIC_EGYPT 0x03 # endif # ifndef SUBLANG_ARABIC_LIBYA # define SUBLANG_ARABIC_LIBYA 0x04 # endif # ifndef SUBLANG_ARABIC_ALGERIA # define SUBLANG_ARABIC_ALGERIA 0x05 # endif # ifndef SUBLANG_ARABIC_MOROCCO # define SUBLANG_ARABIC_MOROCCO 0x06 # endif # ifndef SUBLANG_ARABIC_TUNISIA # define SUBLANG_ARABIC_TUNISIA 0x07 # endif # ifndef SUBLANG_ARABIC_OMAN # define SUBLANG_ARABIC_OMAN 0x08 # endif # ifndef SUBLANG_ARABIC_YEMEN # define SUBLANG_ARABIC_YEMEN 0x09 # endif # ifndef SUBLANG_ARABIC_SYRIA # define SUBLANG_ARABIC_SYRIA 0x0a # endif # ifndef SUBLANG_ARABIC_JORDAN # define SUBLANG_ARABIC_JORDAN 0x0b # endif # ifndef SUBLANG_ARABIC_LEBANON # define SUBLANG_ARABIC_LEBANON 0x0c # endif # ifndef SUBLANG_ARABIC_KUWAIT # define SUBLANG_ARABIC_KUWAIT 0x0d # endif # ifndef SUBLANG_ARABIC_UAE # define SUBLANG_ARABIC_UAE 0x0e # endif # ifndef SUBLANG_ARABIC_BAHRAIN # define SUBLANG_ARABIC_BAHRAIN 0x0f # endif # ifndef SUBLANG_ARABIC_QATAR # define SUBLANG_ARABIC_QATAR 0x10 # endif # ifndef SUBLANG_ARMENIAN_ARMENIA # define SUBLANG_ARMENIAN_ARMENIA 0x01 # endif # ifndef SUBLANG_ASSAMESE_INDIA # define SUBLANG_ASSAMESE_INDIA 0x01 # endif # ifndef SUBLANG_AZERI_LATIN # define SUBLANG_AZERI_LATIN 0x01 # endif # ifndef SUBLANG_AZERI_CYRILLIC # define SUBLANG_AZERI_CYRILLIC 0x02 # endif # ifndef SUBLANG_BASHKIR_RUSSIA # define SUBLANG_BASHKIR_RUSSIA 0x01 # endif # ifndef SUBLANG_BASQUE_BASQUE # define SUBLANG_BASQUE_BASQUE 0x01 # endif # ifndef SUBLANG_BELARUSIAN_BELARUS # define SUBLANG_BELARUSIAN_BELARUS 0x01 # endif # ifndef SUBLANG_BENGALI_INDIA # define SUBLANG_BENGALI_INDIA 0x01 # endif # ifndef SUBLANG_BENGALI_BANGLADESH # define SUBLANG_BENGALI_BANGLADESH 0x02 # endif # ifndef SUBLANG_BOSNIAN_BOSNIA_HERZEGOVINA_LATIN # define SUBLANG_BOSNIAN_BOSNIA_HERZEGOVINA_LATIN 0x05 # endif # ifndef SUBLANG_BOSNIAN_BOSNIA_HERZEGOVINA_CYRILLIC # define SUBLANG_BOSNIAN_BOSNIA_HERZEGOVINA_CYRILLIC 0x08 # endif # ifndef SUBLANG_BRETON_FRANCE # define SUBLANG_BRETON_FRANCE 0x01 # endif # ifndef SUBLANG_BULGARIAN_BULGARIA # define SUBLANG_BULGARIAN_BULGARIA 0x01 # endif # ifndef SUBLANG_CAMBODIAN_CAMBODIA # define SUBLANG_CAMBODIAN_CAMBODIA 0x01 # endif # ifndef SUBLANG_CATALAN_SPAIN # define SUBLANG_CATALAN_SPAIN 0x01 # endif # ifndef SUBLANG_CORSICAN_FRANCE # define SUBLANG_CORSICAN_FRANCE 0x01 # endif # ifndef SUBLANG_CROATIAN_CROATIA # define SUBLANG_CROATIAN_CROATIA 0x01 # endif # ifndef SUBLANG_CROATIAN_BOSNIA_HERZEGOVINA_LATIN # define SUBLANG_CROATIAN_BOSNIA_HERZEGOVINA_LATIN 0x04 # endif # ifndef SUBLANG_CHINESE_MACAU # define SUBLANG_CHINESE_MACAU 0x05 # endif # ifndef SUBLANG_CZECH_CZECH_REPUBLIC # define SUBLANG_CZECH_CZECH_REPUBLIC 0x01 # endif # ifndef SUBLANG_DANISH_DENMARK # define SUBLANG_DANISH_DENMARK 0x01 # endif # ifndef SUBLANG_DARI_AFGHANISTAN # define SUBLANG_DARI_AFGHANISTAN 0x01 # endif # ifndef SUBLANG_DIVEHI_MALDIVES # define SUBLANG_DIVEHI_MALDIVES 0x01 # endif # ifndef SUBLANG_DUTCH_SURINAM # define SUBLANG_DUTCH_SURINAM 0x03 # endif # ifndef SUBLANG_ENGLISH_SOUTH_AFRICA # define SUBLANG_ENGLISH_SOUTH_AFRICA 0x07 # endif # ifndef SUBLANG_ENGLISH_JAMAICA # define SUBLANG_ENGLISH_JAMAICA 0x08 # endif # ifndef SUBLANG_ENGLISH_CARIBBEAN # define SUBLANG_ENGLISH_CARIBBEAN 0x09 # endif # ifndef SUBLANG_ENGLISH_BELIZE # define SUBLANG_ENGLISH_BELIZE 0x0a # endif # ifndef SUBLANG_ENGLISH_TRINIDAD # define SUBLANG_ENGLISH_TRINIDAD 0x0b # endif # ifndef SUBLANG_ENGLISH_ZIMBABWE # define SUBLANG_ENGLISH_ZIMBABWE 0x0c # endif # ifndef SUBLANG_ENGLISH_PHILIPPINES # define SUBLANG_ENGLISH_PHILIPPINES 0x0d # endif # ifndef SUBLANG_ENGLISH_INDONESIA # define SUBLANG_ENGLISH_INDONESIA 0x0e # endif # ifndef SUBLANG_ENGLISH_HONGKONG # define SUBLANG_ENGLISH_HONGKONG 0x0f # endif # ifndef SUBLANG_ENGLISH_INDIA # define SUBLANG_ENGLISH_INDIA 0x10 # endif # ifndef SUBLANG_ENGLISH_MALAYSIA # define SUBLANG_ENGLISH_MALAYSIA 0x11 # endif # ifndef SUBLANG_ENGLISH_SINGAPORE # define SUBLANG_ENGLISH_SINGAPORE 0x12 # endif # ifndef SUBLANG_ESTONIAN_ESTONIA # define SUBLANG_ESTONIAN_ESTONIA 0x01 # endif # ifndef SUBLANG_FAEROESE_FAROE_ISLANDS # define SUBLANG_FAEROESE_FAROE_ISLANDS 0x01 # endif # ifndef SUBLANG_FARSI_IRAN # define SUBLANG_FARSI_IRAN 0x01 # endif # ifndef SUBLANG_FINNISH_FINLAND # define SUBLANG_FINNISH_FINLAND 0x01 # endif # ifndef SUBLANG_FRENCH_LUXEMBOURG # define SUBLANG_FRENCH_LUXEMBOURG 0x05 # endif # ifndef SUBLANG_FRENCH_MONACO # define SUBLANG_FRENCH_MONACO 0x06 # endif # ifndef SUBLANG_FRENCH_WESTINDIES # define SUBLANG_FRENCH_WESTINDIES 0x07 # endif # ifndef SUBLANG_FRENCH_REUNION # define SUBLANG_FRENCH_REUNION 0x08 # endif # ifndef SUBLANG_FRENCH_CONGO # define SUBLANG_FRENCH_CONGO 0x09 # endif # ifndef SUBLANG_FRENCH_SENEGAL # define SUBLANG_FRENCH_SENEGAL 0x0a # endif # ifndef SUBLANG_FRENCH_CAMEROON # define SUBLANG_FRENCH_CAMEROON 0x0b # endif # ifndef SUBLANG_FRENCH_COTEDIVOIRE # define SUBLANG_FRENCH_COTEDIVOIRE 0x0c # endif # ifndef SUBLANG_FRENCH_MALI # define SUBLANG_FRENCH_MALI 0x0d # endif # ifndef SUBLANG_FRENCH_MOROCCO # define SUBLANG_FRENCH_MOROCCO 0x0e # endif # ifndef SUBLANG_FRENCH_HAITI # define SUBLANG_FRENCH_HAITI 0x0f # endif # ifndef SUBLANG_FRISIAN_NETHERLANDS # define SUBLANG_FRISIAN_NETHERLANDS 0x01 # endif # ifndef SUBLANG_GALICIAN_SPAIN # define SUBLANG_GALICIAN_SPAIN 0x01 # endif # ifndef SUBLANG_GEORGIAN_GEORGIA # define SUBLANG_GEORGIAN_GEORGIA 0x01 # endif # ifndef SUBLANG_GERMAN_LUXEMBOURG # define SUBLANG_GERMAN_LUXEMBOURG 0x04 # endif # ifndef SUBLANG_GERMAN_LIECHTENSTEIN # define SUBLANG_GERMAN_LIECHTENSTEIN 0x05 # endif # ifndef SUBLANG_GREEK_GREECE # define SUBLANG_GREEK_GREECE 0x01 # endif # ifndef SUBLANG_GREENLANDIC_GREENLAND # define SUBLANG_GREENLANDIC_GREENLAND 0x01 # endif # ifndef SUBLANG_GUJARATI_INDIA # define SUBLANG_GUJARATI_INDIA 0x01 # endif # ifndef SUBLANG_HAUSA_NIGERIA_LATIN # define SUBLANG_HAUSA_NIGERIA_LATIN 0x01 # endif # ifndef SUBLANG_HEBREW_ISRAEL # define SUBLANG_HEBREW_ISRAEL 0x01 # endif # ifndef SUBLANG_HINDI_INDIA # define SUBLANG_HINDI_INDIA 0x01 # endif # ifndef SUBLANG_HUNGARIAN_HUNGARY # define SUBLANG_HUNGARIAN_HUNGARY 0x01 # endif # ifndef SUBLANG_ICELANDIC_ICELAND # define SUBLANG_ICELANDIC_ICELAND 0x01 # endif # ifndef SUBLANG_IGBO_NIGERIA # define SUBLANG_IGBO_NIGERIA 0x01 # endif # ifndef SUBLANG_INDONESIAN_INDONESIA # define SUBLANG_INDONESIAN_INDONESIA 0x01 # endif # ifndef SUBLANG_INUKTITUT_CANADA # define SUBLANG_INUKTITUT_CANADA 0x01 # endif # undef SUBLANG_INUKTITUT_CANADA_LATIN # define SUBLANG_INUKTITUT_CANADA_LATIN 0x02 # undef SUBLANG_IRISH_IRELAND # define SUBLANG_IRISH_IRELAND 0x02 # ifndef SUBLANG_JAPANESE_JAPAN # define SUBLANG_JAPANESE_JAPAN 0x01 # endif # ifndef SUBLANG_KANNADA_INDIA # define SUBLANG_KANNADA_INDIA 0x01 # endif # ifndef SUBLANG_KASHMIRI_INDIA # define SUBLANG_KASHMIRI_INDIA 0x02 # endif # ifndef SUBLANG_KAZAK_KAZAKHSTAN # define SUBLANG_KAZAK_KAZAKHSTAN 0x01 # endif # ifndef SUBLANG_KICHE_GUATEMALA # define SUBLANG_KICHE_GUATEMALA 0x01 # endif # ifndef SUBLANG_KINYARWANDA_RWANDA # define SUBLANG_KINYARWANDA_RWANDA 0x01 # endif # ifndef SUBLANG_KONKANI_INDIA # define SUBLANG_KONKANI_INDIA 0x01 # endif # ifndef SUBLANG_KYRGYZ_KYRGYZSTAN # define SUBLANG_KYRGYZ_KYRGYZSTAN 0x01 # endif # ifndef SUBLANG_LAO_LAOS # define SUBLANG_LAO_LAOS 0x01 # endif # ifndef SUBLANG_LATVIAN_LATVIA # define SUBLANG_LATVIAN_LATVIA 0x01 # endif # ifndef SUBLANG_LITHUANIAN_LITHUANIA # define SUBLANG_LITHUANIAN_LITHUANIA 0x01 # endif # undef SUBLANG_LOWER_SORBIAN_GERMANY # define SUBLANG_LOWER_SORBIAN_GERMANY 0x02 # ifndef SUBLANG_LUXEMBOURGISH_LUXEMBOURG # define SUBLANG_LUXEMBOURGISH_LUXEMBOURG 0x01 # endif # ifndef SUBLANG_MACEDONIAN_MACEDONIA # define SUBLANG_MACEDONIAN_MACEDONIA 0x01 # endif # ifndef SUBLANG_MALAY_MALAYSIA # define SUBLANG_MALAY_MALAYSIA 0x01 # endif # ifndef SUBLANG_MALAY_BRUNEI_DARUSSALAM # define SUBLANG_MALAY_BRUNEI_DARUSSALAM 0x02 # endif # ifndef SUBLANG_MALAYALAM_INDIA # define SUBLANG_MALAYALAM_INDIA 0x01 # endif # ifndef SUBLANG_MALTESE_MALTA # define SUBLANG_MALTESE_MALTA 0x01 # endif # ifndef SUBLANG_MAORI_NEW_ZEALAND # define SUBLANG_MAORI_NEW_ZEALAND 0x01 # endif # ifndef SUBLANG_MAPUDUNGUN_CHILE # define SUBLANG_MAPUDUNGUN_CHILE 0x01 # endif # ifndef SUBLANG_MARATHI_INDIA # define SUBLANG_MARATHI_INDIA 0x01 # endif # ifndef SUBLANG_MOHAWK_CANADA # define SUBLANG_MOHAWK_CANADA 0x01 # endif # ifndef SUBLANG_MONGOLIAN_CYRILLIC_MONGOLIA # define SUBLANG_MONGOLIAN_CYRILLIC_MONGOLIA 0x01 # endif # ifndef SUBLANG_MONGOLIAN_PRC # define SUBLANG_MONGOLIAN_PRC 0x02 # endif # ifndef SUBLANG_NEPALI_NEPAL # define SUBLANG_NEPALI_NEPAL 0x01 # endif # ifndef SUBLANG_NEPALI_INDIA # define SUBLANG_NEPALI_INDIA 0x02 # endif # ifndef SUBLANG_OCCITAN_FRANCE # define SUBLANG_OCCITAN_FRANCE 0x01 # endif # ifndef SUBLANG_ORIYA_INDIA # define SUBLANG_ORIYA_INDIA 0x01 # endif # ifndef SUBLANG_PASHTO_AFGHANISTAN # define SUBLANG_PASHTO_AFGHANISTAN 0x01 # endif # ifndef SUBLANG_POLISH_POLAND # define SUBLANG_POLISH_POLAND 0x01 # endif # ifndef SUBLANG_PUNJABI_INDIA # define SUBLANG_PUNJABI_INDIA 0x01 # endif # ifndef SUBLANG_PUNJABI_PAKISTAN # define SUBLANG_PUNJABI_PAKISTAN 0x02 # endif # ifndef SUBLANG_QUECHUA_BOLIVIA # define SUBLANG_QUECHUA_BOLIVIA 0x01 # endif # ifndef SUBLANG_QUECHUA_ECUADOR # define SUBLANG_QUECHUA_ECUADOR 0x02 # endif # ifndef SUBLANG_QUECHUA_PERU # define SUBLANG_QUECHUA_PERU 0x03 # endif # ifndef SUBLANG_ROMANIAN_ROMANIA # define SUBLANG_ROMANIAN_ROMANIA 0x01 # endif # ifndef SUBLANG_ROMANIAN_MOLDOVA # define SUBLANG_ROMANIAN_MOLDOVA 0x02 # endif # ifndef SUBLANG_ROMANSH_SWITZERLAND # define SUBLANG_ROMANSH_SWITZERLAND 0x01 # endif # ifndef SUBLANG_RUSSIAN_RUSSIA # define SUBLANG_RUSSIAN_RUSSIA 0x01 # endif # ifndef SUBLANG_RUSSIAN_MOLDAVIA # define SUBLANG_RUSSIAN_MOLDAVIA 0x02 # endif # ifndef SUBLANG_SAMI_NORTHERN_NORWAY # define SUBLANG_SAMI_NORTHERN_NORWAY 0x01 # endif # ifndef SUBLANG_SAMI_NORTHERN_SWEDEN # define SUBLANG_SAMI_NORTHERN_SWEDEN 0x02 # endif # ifndef SUBLANG_SAMI_NORTHERN_FINLAND # define SUBLANG_SAMI_NORTHERN_FINLAND 0x03 # endif # ifndef SUBLANG_SAMI_LULE_NORWAY # define SUBLANG_SAMI_LULE_NORWAY 0x04 # endif # ifndef SUBLANG_SAMI_LULE_SWEDEN # define SUBLANG_SAMI_LULE_SWEDEN 0x05 # endif # ifndef SUBLANG_SAMI_SOUTHERN_NORWAY # define SUBLANG_SAMI_SOUTHERN_NORWAY 0x06 # endif # ifndef SUBLANG_SAMI_SOUTHERN_SWEDEN # define SUBLANG_SAMI_SOUTHERN_SWEDEN 0x07 # endif # undef SUBLANG_SAMI_SKOLT_FINLAND # define SUBLANG_SAMI_SKOLT_FINLAND 0x08 # undef SUBLANG_SAMI_INARI_FINLAND # define SUBLANG_SAMI_INARI_FINLAND 0x09 # ifndef SUBLANG_SANSKRIT_INDIA # define SUBLANG_SANSKRIT_INDIA 0x01 # endif # ifndef SUBLANG_SERBIAN_LATIN # define SUBLANG_SERBIAN_LATIN 0x02 # endif # ifndef SUBLANG_SERBIAN_CYRILLIC # define SUBLANG_SERBIAN_CYRILLIC 0x03 # endif # ifndef SUBLANG_SINDHI_INDIA # define SUBLANG_SINDHI_INDIA 0x01 # endif # undef SUBLANG_SINDHI_PAKISTAN # define SUBLANG_SINDHI_PAKISTAN 0x02 # ifndef SUBLANG_SINDHI_AFGHANISTAN # define SUBLANG_SINDHI_AFGHANISTAN 0x02 # endif # ifndef SUBLANG_SINHALESE_SRI_LANKA # define SUBLANG_SINHALESE_SRI_LANKA 0x01 # endif # ifndef SUBLANG_SLOVAK_SLOVAKIA # define SUBLANG_SLOVAK_SLOVAKIA 0x01 # endif # ifndef SUBLANG_SLOVENIAN_SLOVENIA # define SUBLANG_SLOVENIAN_SLOVENIA 0x01 # endif # ifndef SUBLANG_SOTHO_SOUTH_AFRICA # define SUBLANG_SOTHO_SOUTH_AFRICA 0x01 # endif # ifndef SUBLANG_SPANISH_GUATEMALA # define SUBLANG_SPANISH_GUATEMALA 0x04 # endif # ifndef SUBLANG_SPANISH_COSTA_RICA # define SUBLANG_SPANISH_COSTA_RICA 0x05 # endif # ifndef SUBLANG_SPANISH_PANAMA # define SUBLANG_SPANISH_PANAMA 0x06 # endif # ifndef SUBLANG_SPANISH_DOMINICAN_REPUBLIC # define SUBLANG_SPANISH_DOMINICAN_REPUBLIC 0x07 # endif # ifndef SUBLANG_SPANISH_VENEZUELA # define SUBLANG_SPANISH_VENEZUELA 0x08 # endif # ifndef SUBLANG_SPANISH_COLOMBIA # define SUBLANG_SPANISH_COLOMBIA 0x09 # endif # ifndef SUBLANG_SPANISH_PERU # define SUBLANG_SPANISH_PERU 0x0a # endif # ifndef SUBLANG_SPANISH_ARGENTINA # define SUBLANG_SPANISH_ARGENTINA 0x0b # endif # ifndef SUBLANG_SPANISH_ECUADOR # define SUBLANG_SPANISH_ECUADOR 0x0c # endif # ifndef SUBLANG_SPANISH_CHILE # define SUBLANG_SPANISH_CHILE 0x0d # endif # ifndef SUBLANG_SPANISH_URUGUAY # define SUBLANG_SPANISH_URUGUAY 0x0e # endif # ifndef SUBLANG_SPANISH_PARAGUAY # define SUBLANG_SPANISH_PARAGUAY 0x0f # endif # ifndef SUBLANG_SPANISH_BOLIVIA # define SUBLANG_SPANISH_BOLIVIA 0x10 # endif # ifndef SUBLANG_SPANISH_EL_SALVADOR # define SUBLANG_SPANISH_EL_SALVADOR 0x11 # endif # ifndef SUBLANG_SPANISH_HONDURAS # define SUBLANG_SPANISH_HONDURAS 0x12 # endif # ifndef SUBLANG_SPANISH_NICARAGUA # define SUBLANG_SPANISH_NICARAGUA 0x13 # endif # ifndef SUBLANG_SPANISH_PUERTO_RICO # define SUBLANG_SPANISH_PUERTO_RICO 0x14 # endif # ifndef SUBLANG_SPANISH_US # define SUBLANG_SPANISH_US 0x15 # endif # ifndef SUBLANG_SWAHILI_KENYA # define SUBLANG_SWAHILI_KENYA 0x01 # endif # ifndef SUBLANG_SWEDISH_SWEDEN # define SUBLANG_SWEDISH_SWEDEN 0x01 # endif # ifndef SUBLANG_SWEDISH_FINLAND # define SUBLANG_SWEDISH_FINLAND 0x02 # endif # ifndef SUBLANG_SYRIAC_SYRIA # define SUBLANG_SYRIAC_SYRIA 0x01 # endif # ifndef SUBLANG_TAGALOG_PHILIPPINES # define SUBLANG_TAGALOG_PHILIPPINES 0x01 # endif # ifndef SUBLANG_TAJIK_TAJIKISTAN # define SUBLANG_TAJIK_TAJIKISTAN 0x01 # endif # ifndef SUBLANG_TAMAZIGHT_ARABIC # define SUBLANG_TAMAZIGHT_ARABIC 0x01 # endif # ifndef SUBLANG_TAMAZIGHT_ALGERIA_LATIN # define SUBLANG_TAMAZIGHT_ALGERIA_LATIN 0x02 # endif # ifndef SUBLANG_TAMIL_INDIA # define SUBLANG_TAMIL_INDIA 0x01 # endif # ifndef SUBLANG_TATAR_RUSSIA # define SUBLANG_TATAR_RUSSIA 0x01 # endif # ifndef SUBLANG_TELUGU_INDIA # define SUBLANG_TELUGU_INDIA 0x01 # endif # ifndef SUBLANG_THAI_THAILAND # define SUBLANG_THAI_THAILAND 0x01 # endif # ifndef SUBLANG_TIBETAN_PRC # define SUBLANG_TIBETAN_PRC 0x01 # endif # undef SUBLANG_TIBETAN_BHUTAN # define SUBLANG_TIBETAN_BHUTAN 0x02 # ifndef SUBLANG_TIGRINYA_ETHIOPIA # define SUBLANG_TIGRINYA_ETHIOPIA 0x01 # endif # ifndef SUBLANG_TIGRINYA_ERITREA # define SUBLANG_TIGRINYA_ERITREA 0x02 # endif # ifndef SUBLANG_TSWANA_SOUTH_AFRICA # define SUBLANG_TSWANA_SOUTH_AFRICA 0x01 # endif # ifndef SUBLANG_TURKISH_TURKEY # define SUBLANG_TURKISH_TURKEY 0x01 # endif # ifndef SUBLANG_TURKMEN_TURKMENISTAN # define SUBLANG_TURKMEN_TURKMENISTAN 0x01 # endif # ifndef SUBLANG_UIGHUR_PRC # define SUBLANG_UIGHUR_PRC 0x01 # endif # ifndef SUBLANG_UKRAINIAN_UKRAINE # define SUBLANG_UKRAINIAN_UKRAINE 0x01 # endif # ifndef SUBLANG_UPPER_SORBIAN_GERMANY # define SUBLANG_UPPER_SORBIAN_GERMANY 0x01 # endif # ifndef SUBLANG_URDU_PAKISTAN # define SUBLANG_URDU_PAKISTAN 0x01 # endif # ifndef SUBLANG_URDU_INDIA # define SUBLANG_URDU_INDIA 0x02 # endif # ifndef SUBLANG_UZBEK_LATIN # define SUBLANG_UZBEK_LATIN 0x01 # endif # ifndef SUBLANG_UZBEK_CYRILLIC # define SUBLANG_UZBEK_CYRILLIC 0x02 # endif # ifndef SUBLANG_VIETNAMESE_VIETNAM # define SUBLANG_VIETNAMESE_VIETNAM 0x01 # endif # ifndef SUBLANG_WELSH_UNITED_KINGDOM # define SUBLANG_WELSH_UNITED_KINGDOM 0x01 # endif # ifndef SUBLANG_WOLOF_SENEGAL # define SUBLANG_WOLOF_SENEGAL 0x01 # endif # ifndef SUBLANG_XHOSA_SOUTH_AFRICA # define SUBLANG_XHOSA_SOUTH_AFRICA 0x01 # endif # ifndef SUBLANG_YAKUT_RUSSIA # define SUBLANG_YAKUT_RUSSIA 0x01 # endif # ifndef SUBLANG_YI_PRC # define SUBLANG_YI_PRC 0x01 # endif # ifndef SUBLANG_YORUBA_NIGERIA # define SUBLANG_YORUBA_NIGERIA 0x01 # endif # ifndef SUBLANG_ZULU_SOUTH_AFRICA # define SUBLANG_ZULU_SOUTH_AFRICA 0x01 # endif /* GetLocaleInfoA operations. */ # ifndef LOCALE_SNAME # define LOCALE_SNAME 0x5c # endif # ifndef LOCALE_NAME_MAX_LENGTH # define LOCALE_NAME_MAX_LENGTH 85 # endif #endif #if HAVE_CFLOCALECOPYCURRENT || HAVE_CFPREFERENCESCOPYAPPVALUE /* Mac OS X 10.2 or newer */ /* Canonicalize a Mac OS X locale name to a Unix locale name. NAME is a sufficiently large buffer. On input, it contains the Mac OS X locale name. On output, it contains the Unix locale name. */ # if !defined IN_LIBINTL static # endif void gl_locale_name_canonicalize (char *name) { /* This conversion is based on a posting by Deborah GoldSmith on 2005-03-08, http://lists.apple.com/archives/carbon-dev/2005/Mar/msg00293.html */ /* Convert legacy (NeXTstep inherited) English names to Unix (ISO 639 and ISO 3166) names. Prior to Mac OS X 10.3, there is no API for doing this. Therefore we do it ourselves, using a table based on the results of the Mac OS X 10.3.8 function CFLocaleCreateCanonicalLocaleIdentifierFromString(). */ typedef struct { const char legacy[21+1]; const char unixy[5+1]; } legacy_entry; static const legacy_entry legacy_table[] = { { "Afrikaans", "af" }, { "Albanian", "sq" }, { "Amharic", "am" }, { "Arabic", "ar" }, { "Armenian", "hy" }, { "Assamese", "as" }, { "Aymara", "ay" }, { "Azerbaijani", "az" }, { "Basque", "eu" }, { "Belarusian", "be" }, { "Belorussian", "be" }, { "Bengali", "bn" }, { "Brazilian Portugese", "pt_BR" }, { "Brazilian Portuguese", "pt_BR" }, { "Breton", "br" }, { "Bulgarian", "bg" }, { "Burmese", "my" }, { "Byelorussian", "be" }, { "Catalan", "ca" }, { "Chewa", "ny" }, { "Chichewa", "ny" }, { "Chinese", "zh" }, { "Chinese, Simplified", "zh_CN" }, { "Chinese, Traditional", "zh_TW" }, { "Chinese, Tradtional", "zh_TW" }, { "Croatian", "hr" }, { "Czech", "cs" }, { "Danish", "da" }, { "Dutch", "nl" }, { "Dzongkha", "dz" }, { "English", "en" }, { "Esperanto", "eo" }, { "Estonian", "et" }, { "Faroese", "fo" }, { "Farsi", "fa" }, { "Finnish", "fi" }, { "Flemish", "nl_BE" }, { "French", "fr" }, { "Galician", "gl" }, { "Gallegan", "gl" }, { "Georgian", "ka" }, { "German", "de" }, { "Greek", "el" }, { "Greenlandic", "kl" }, { "Guarani", "gn" }, { "Gujarati", "gu" }, { "Hawaiian", "haw" }, /* Yes, "haw", not "cpe". */ { "Hebrew", "he" }, { "Hindi", "hi" }, { "Hungarian", "hu" }, { "Icelandic", "is" }, { "Indonesian", "id" }, { "Inuktitut", "iu" }, { "Irish", "ga" }, { "Italian", "it" }, { "Japanese", "ja" }, { "Javanese", "jv" }, { "Kalaallisut", "kl" }, { "Kannada", "kn" }, { "Kashmiri", "ks" }, { "Kazakh", "kk" }, { "Khmer", "km" }, { "Kinyarwanda", "rw" }, { "Kirghiz", "ky" }, { "Korean", "ko" }, { "Kurdish", "ku" }, { "Latin", "la" }, { "Latvian", "lv" }, { "Lithuanian", "lt" }, { "Macedonian", "mk" }, { "Malagasy", "mg" }, { "Malay", "ms" }, { "Malayalam", "ml" }, { "Maltese", "mt" }, { "Manx", "gv" }, { "Marathi", "mr" }, { "Moldavian", "mo" }, { "Mongolian", "mn" }, { "Nepali", "ne" }, { "Norwegian", "nb" }, /* Yes, "nb", not the obsolete "no". */ { "Nyanja", "ny" }, { "Nynorsk", "nn" }, { "Oriya", "or" }, { "Oromo", "om" }, { "Panjabi", "pa" }, { "Pashto", "ps" }, { "Persian", "fa" }, { "Polish", "pl" }, { "Portuguese", "pt" }, { "Portuguese, Brazilian", "pt_BR" }, { "Punjabi", "pa" }, { "Pushto", "ps" }, { "Quechua", "qu" }, { "Romanian", "ro" }, { "Ruanda", "rw" }, { "Rundi", "rn" }, { "Russian", "ru" }, { "Sami", "se_NO" }, /* Not just "se". */ { "Sanskrit", "sa" }, { "Scottish", "gd" }, { "Serbian", "sr" }, { "Simplified Chinese", "zh_CN" }, { "Sindhi", "sd" }, { "Sinhalese", "si" }, { "Slovak", "sk" }, { "Slovenian", "sl" }, { "Somali", "so" }, { "Spanish", "es" }, { "Sundanese", "su" }, { "Swahili", "sw" }, { "Swedish", "sv" }, { "Tagalog", "tl" }, { "Tajik", "tg" }, { "Tajiki", "tg" }, { "Tamil", "ta" }, { "Tatar", "tt" }, { "Telugu", "te" }, { "Thai", "th" }, { "Tibetan", "bo" }, { "Tigrinya", "ti" }, { "Tongan", "to" }, { "Traditional Chinese", "zh_TW" }, { "Turkish", "tr" }, { "Turkmen", "tk" }, { "Uighur", "ug" }, { "Ukrainian", "uk" }, { "Urdu", "ur" }, { "Uzbek", "uz" }, { "Vietnamese", "vi" }, { "Welsh", "cy" }, { "Yiddish", "yi" } }; /* Convert new-style locale names with language tags (ISO 639 and ISO 15924) to Unix (ISO 639 and ISO 3166) names. */ typedef struct { const char langtag[7+1]; const char unixy[12+1]; } langtag_entry; static const langtag_entry langtag_table[] = { /* Mac OS X has "az-Arab", "az-Cyrl", "az-Latn". The default script for az on Unix is Latin. */ { "az-Latn", "az" }, /* Mac OS X has "ga-dots". Does not yet exist on Unix. */ { "ga-dots", "ga" }, /* Mac OS X has "kk-Cyrl". Does not yet exist on Unix. */ /* Mac OS X has "mn-Cyrl", "mn-Mong". The default script for mn on Unix is Cyrillic. */ { "mn-Cyrl", "mn" }, /* Mac OS X has "ms-Arab", "ms-Latn". The default script for ms on Unix is Latin. */ { "ms-Latn", "ms" }, /* Mac OS X has "tg-Cyrl". The default script for tg on Unix is Cyrillic. */ { "tg-Cyrl", "tg" }, /* Mac OS X has "tk-Cyrl". Does not yet exist on Unix. */ /* Mac OS X has "tt-Cyrl". The default script for tt on Unix is Cyrillic. */ { "tt-Cyrl", "tt" }, /* Mac OS X has "zh-Hans", "zh-Hant". Country codes are used to distinguish these on Unix. */ { "zh-Hans", "zh_CN" }, { "zh-Hant", "zh_TW" } }; /* Convert script names (ISO 15924) to Unix conventions. See http://www.unicode.org/iso15924/iso15924-codes.html */ typedef struct { const char script[4+1]; const char unixy[9+1]; } script_entry; static const script_entry script_table[] = { { "Arab", "arabic" }, { "Cyrl", "cyrillic" }, { "Mong", "mongolian" } }; /* Step 1: Convert using legacy_table. */ if (name[0] >= 'A' && name[0] <= 'Z') { unsigned int i1, i2; i1 = 0; i2 = sizeof (legacy_table) / sizeof (legacy_entry); while (i2 - i1 > 1) { /* At this point we know that if name occurs in legacy_table, its index must be >= i1 and < i2. */ unsigned int i = (i1 + i2) >> 1; const legacy_entry *p = &legacy_table[i]; if (strcmp (name, p->legacy) < 0) i2 = i; else i1 = i; } if (strcmp (name, legacy_table[i1].legacy) == 0) { strcpy (name, legacy_table[i1].unixy); return; } } /* Step 2: Convert using langtag_table and script_table. */ if (strlen (name) == 7 && name[2] == '-') { unsigned int i1, i2; i1 = 0; i2 = sizeof (langtag_table) / sizeof (langtag_entry); while (i2 - i1 > 1) { /* At this point we know that if name occurs in langtag_table, its index must be >= i1 and < i2. */ unsigned int i = (i1 + i2) >> 1; const langtag_entry *p = &langtag_table[i]; if (strcmp (name, p->langtag) < 0) i2 = i; else i1 = i; } if (strcmp (name, langtag_table[i1].langtag) == 0) { strcpy (name, langtag_table[i1].unixy); return; } i1 = 0; i2 = sizeof (script_table) / sizeof (script_entry); while (i2 - i1 > 1) { /* At this point we know that if (name + 3) occurs in script_table, its index must be >= i1 and < i2. */ unsigned int i = (i1 + i2) >> 1; const script_entry *p = &script_table[i]; if (strcmp (name + 3, p->script) < 0) i2 = i; else i1 = i; } if (strcmp (name + 3, script_table[i1].script) == 0) { name[2] = '@'; strcpy (name + 3, script_table[i1].unixy); return; } } /* Step 3: Convert new-style dash to Unix underscore. */ { char *p; for (p = name; *p != '\0'; p++) if (*p == '-') *p = '_'; } } #endif #if defined WINDOWS_NATIVE || defined __CYGWIN__ /* Native Windows or Cygwin */ /* Canonicalize a Windows native locale name to a Unix locale name. NAME is a sufficiently large buffer. On input, it contains the Windows locale name. On output, it contains the Unix locale name. */ # if !defined IN_LIBINTL static # endif void gl_locale_name_canonicalize (char *name) { /* FIXME: This is probably incomplete: it does not handle "zh-Hans" and "zh-Hant". */ char *p; for (p = name; *p != '\0'; p++) if (*p == '-') { *p = '_'; p++; for (; *p != '\0'; p++) { if (*p >= 'a' && *p <= 'z') *p += 'A' - 'a'; if (*p == '-') { *p = '\0'; return; } } return; } } # if !defined IN_LIBINTL static # endif const char * gl_locale_name_from_win32_LANGID (LANGID langid) { /* Activate the new code only when the GETTEXT_MUI environment variable is set, for the time being, since the new code is not well tested. */ if (getenv ("GETTEXT_MUI") != NULL) { static char namebuf[256]; /* Query the system's notion of locale name. On Windows95/98/ME, GetLocaleInfoA returns some incorrect results. But we don't need to support systems that are so old. */ if (GetLocaleInfoA (MAKELCID (langid, SORT_DEFAULT), LOCALE_SNAME, namebuf, sizeof (namebuf) - 1)) { /* Convert it to a Unix locale name. */ gl_locale_name_canonicalize (namebuf); return namebuf; } } /* Internet Explorer has an LCID to RFC3066 name mapping stored in HKEY_CLASSES_ROOT\Mime\Database\Rfc1766. But we better don't use that since IE's i18n subsystem is known to be inconsistent with the native Windows base (e.g. they have different character conversion facilities that produce different results). */ /* Use our own table. */ { int primary, sub; /* Split into language and territory part. */ primary = PRIMARYLANGID (langid); sub = SUBLANGID (langid); /* Dispatch on language. See also http://www.unicode.org/unicode/onlinedat/languages.html . For details about languages, see http://www.ethnologue.com/ . */ switch (primary) { case LANG_AFRIKAANS: switch (sub) { case SUBLANG_AFRIKAANS_SOUTH_AFRICA: return "af_ZA"; } return "af"; case LANG_ALBANIAN: switch (sub) { case SUBLANG_ALBANIAN_ALBANIA: return "sq_AL"; } return "sq"; case LANG_ALSATIAN: switch (sub) { case SUBLANG_ALSATIAN_FRANCE: return "gsw_FR"; } return "gsw"; case LANG_AMHARIC: switch (sub) { case SUBLANG_AMHARIC_ETHIOPIA: return "am_ET"; } return "am"; case LANG_ARABIC: switch (sub) { case SUBLANG_ARABIC_SAUDI_ARABIA: return "ar_SA"; case SUBLANG_ARABIC_IRAQ: return "ar_IQ"; case SUBLANG_ARABIC_EGYPT: return "ar_EG"; case SUBLANG_ARABIC_LIBYA: return "ar_LY"; case SUBLANG_ARABIC_ALGERIA: return "ar_DZ"; case SUBLANG_ARABIC_MOROCCO: return "ar_MA"; case SUBLANG_ARABIC_TUNISIA: return "ar_TN"; case SUBLANG_ARABIC_OMAN: return "ar_OM"; case SUBLANG_ARABIC_YEMEN: return "ar_YE"; case SUBLANG_ARABIC_SYRIA: return "ar_SY"; case SUBLANG_ARABIC_JORDAN: return "ar_JO"; case SUBLANG_ARABIC_LEBANON: return "ar_LB"; case SUBLANG_ARABIC_KUWAIT: return "ar_KW"; case SUBLANG_ARABIC_UAE: return "ar_AE"; case SUBLANG_ARABIC_BAHRAIN: return "ar_BH"; case SUBLANG_ARABIC_QATAR: return "ar_QA"; } return "ar"; case LANG_ARMENIAN: switch (sub) { case SUBLANG_ARMENIAN_ARMENIA: return "hy_AM"; } return "hy"; case LANG_ASSAMESE: switch (sub) { case SUBLANG_ASSAMESE_INDIA: return "as_IN"; } return "as"; case LANG_AZERI: switch (sub) { /* FIXME: Adjust this when Azerbaijani locales appear on Unix. */ case 0x1e: return "az@latin"; case SUBLANG_AZERI_LATIN: return "az_AZ@latin"; case 0x1d: return "az@cyrillic"; case SUBLANG_AZERI_CYRILLIC: return "az_AZ@cyrillic"; } return "az"; case LANG_BASHKIR: switch (sub) { case SUBLANG_BASHKIR_RUSSIA: return "ba_RU"; } return "ba"; case LANG_BASQUE: switch (sub) { case SUBLANG_BASQUE_BASQUE: return "eu_ES"; } return "eu"; /* Ambiguous: could be "eu_ES" or "eu_FR". */ case LANG_BELARUSIAN: switch (sub) { case SUBLANG_BELARUSIAN_BELARUS: return "be_BY"; } return "be"; case LANG_BENGALI: switch (sub) { case SUBLANG_BENGALI_INDIA: return "bn_IN"; case SUBLANG_BENGALI_BANGLADESH: return "bn_BD"; } return "bn"; case LANG_BRETON: switch (sub) { case SUBLANG_BRETON_FRANCE: return "br_FR"; } return "br"; case LANG_BULGARIAN: switch (sub) { case SUBLANG_BULGARIAN_BULGARIA: return "bg_BG"; } return "bg"; case LANG_BURMESE: switch (sub) { case SUBLANG_DEFAULT: return "my_MM"; } return "my"; case LANG_CAMBODIAN: switch (sub) { case SUBLANG_CAMBODIAN_CAMBODIA: return "km_KH"; } return "km"; case LANG_CATALAN: switch (sub) { case SUBLANG_CATALAN_SPAIN: return "ca_ES"; } return "ca"; case LANG_CHEROKEE: switch (sub) { case SUBLANG_DEFAULT: return "chr_US"; } return "chr"; case LANG_CHINESE: switch (sub) { case SUBLANG_CHINESE_TRADITIONAL: case 0x1f: return "zh_TW"; case SUBLANG_CHINESE_SIMPLIFIED: case 0x00: return "zh_CN"; case SUBLANG_CHINESE_HONGKONG: return "zh_HK"; /* traditional */ case SUBLANG_CHINESE_SINGAPORE: return "zh_SG"; /* simplified */ case SUBLANG_CHINESE_MACAU: return "zh_MO"; /* traditional */ } return "zh"; case LANG_CORSICAN: switch (sub) { case SUBLANG_CORSICAN_FRANCE: return "co_FR"; } return "co"; case LANG_CROATIAN: /* LANG_CROATIAN == LANG_SERBIAN == LANG_BOSNIAN * What used to be called Serbo-Croatian * should really now be two separate * languages because of political reasons. * (Says tml, who knows nothing about Serbian * or Croatian.) * (I can feel those flames coming already.) */ switch (sub) { /* Croatian */ case 0x00: return "hr"; case SUBLANG_CROATIAN_CROATIA: return "hr_HR"; case SUBLANG_CROATIAN_BOSNIA_HERZEGOVINA_LATIN: return "hr_BA"; /* Serbian */ case 0x1f: return "sr"; case 0x1c: return "sr"; /* latin */ case SUBLANG_SERBIAN_LATIN: return "sr_CS"; /* latin */ case 0x09: return "sr_RS"; /* latin */ case 0x0b: return "sr_ME"; /* latin */ case 0x06: return "sr_BA"; /* latin */ case 0x1b: return "sr@cyrillic"; case SUBLANG_SERBIAN_CYRILLIC: return "sr_CS@cyrillic"; case 0x0a: return "sr_RS@cyrillic"; case 0x0c: return "sr_ME@cyrillic"; case 0x07: return "sr_BA@cyrillic"; /* Bosnian */ case 0x1e: return "bs"; case 0x1a: return "bs"; /* latin */ case SUBLANG_BOSNIAN_BOSNIA_HERZEGOVINA_LATIN: return "bs_BA"; /* latin */ case 0x19: return "bs@cyrillic"; case SUBLANG_BOSNIAN_BOSNIA_HERZEGOVINA_CYRILLIC: return "bs_BA@cyrillic"; } return "hr"; case LANG_CZECH: switch (sub) { case SUBLANG_CZECH_CZECH_REPUBLIC: return "cs_CZ"; } return "cs"; case LANG_DANISH: switch (sub) { case SUBLANG_DANISH_DENMARK: return "da_DK"; } return "da"; case LANG_DARI: /* FIXME: Adjust this when such locales appear on Unix. */ switch (sub) { case SUBLANG_DARI_AFGHANISTAN: return "prs_AF"; } return "prs"; case LANG_DIVEHI: switch (sub) { case SUBLANG_DIVEHI_MALDIVES: return "dv_MV"; } return "dv"; case LANG_DUTCH: switch (sub) { case SUBLANG_DUTCH: return "nl_NL"; case SUBLANG_DUTCH_BELGIAN: /* FLEMISH, VLAAMS */ return "nl_BE"; case SUBLANG_DUTCH_SURINAM: return "nl_SR"; } return "nl"; case LANG_EDO: switch (sub) { case SUBLANG_DEFAULT: return "bin_NG"; } return "bin"; case LANG_ENGLISH: switch (sub) { /* SUBLANG_ENGLISH_US == SUBLANG_DEFAULT. Heh. I thought * English was the language spoken in England. * Oh well. */ case SUBLANG_ENGLISH_US: return "en_US"; case SUBLANG_ENGLISH_UK: return "en_GB"; case SUBLANG_ENGLISH_AUS: return "en_AU"; case SUBLANG_ENGLISH_CAN: return "en_CA"; case SUBLANG_ENGLISH_NZ: return "en_NZ"; case SUBLANG_ENGLISH_EIRE: return "en_IE"; case SUBLANG_ENGLISH_SOUTH_AFRICA: return "en_ZA"; case SUBLANG_ENGLISH_JAMAICA: return "en_JM"; case SUBLANG_ENGLISH_CARIBBEAN: return "en_GD"; /* Grenada? */ case SUBLANG_ENGLISH_BELIZE: return "en_BZ"; case SUBLANG_ENGLISH_TRINIDAD: return "en_TT"; case SUBLANG_ENGLISH_ZIMBABWE: return "en_ZW"; case SUBLANG_ENGLISH_PHILIPPINES: return "en_PH"; case SUBLANG_ENGLISH_INDONESIA: return "en_ID"; case SUBLANG_ENGLISH_HONGKONG: return "en_HK"; case SUBLANG_ENGLISH_INDIA: return "en_IN"; case SUBLANG_ENGLISH_MALAYSIA: return "en_MY"; case SUBLANG_ENGLISH_SINGAPORE: return "en_SG"; } return "en"; case LANG_ESTONIAN: switch (sub) { case SUBLANG_ESTONIAN_ESTONIA: return "et_EE"; } return "et"; case LANG_FAEROESE: switch (sub) { case SUBLANG_FAEROESE_FAROE_ISLANDS: return "fo_FO"; } return "fo"; case LANG_FARSI: switch (sub) { case SUBLANG_FARSI_IRAN: return "fa_IR"; } return "fa"; case LANG_FINNISH: switch (sub) { case SUBLANG_FINNISH_FINLAND: return "fi_FI"; } return "fi"; case LANG_FRENCH: switch (sub) { case SUBLANG_FRENCH: return "fr_FR"; case SUBLANG_FRENCH_BELGIAN: /* WALLOON */ return "fr_BE"; case SUBLANG_FRENCH_CANADIAN: return "fr_CA"; case SUBLANG_FRENCH_SWISS: return "fr_CH"; case SUBLANG_FRENCH_LUXEMBOURG: return "fr_LU"; case SUBLANG_FRENCH_MONACO: return "fr_MC"; case SUBLANG_FRENCH_WESTINDIES: return "fr"; /* Caribbean? */ case SUBLANG_FRENCH_REUNION: return "fr_RE"; case SUBLANG_FRENCH_CONGO: return "fr_CG"; case SUBLANG_FRENCH_SENEGAL: return "fr_SN"; case SUBLANG_FRENCH_CAMEROON: return "fr_CM"; case SUBLANG_FRENCH_COTEDIVOIRE: return "fr_CI"; case SUBLANG_FRENCH_MALI: return "fr_ML"; case SUBLANG_FRENCH_MOROCCO: return "fr_MA"; case SUBLANG_FRENCH_HAITI: return "fr_HT"; } return "fr"; case LANG_FRISIAN: switch (sub) { case SUBLANG_FRISIAN_NETHERLANDS: return "fy_NL"; } return "fy"; case LANG_FULFULDE: /* Spoken in Nigeria, Guinea, Senegal, Mali, Niger, Cameroon, Benin. */ switch (sub) { case SUBLANG_DEFAULT: return "ff_NG"; } return "ff"; case LANG_GAELIC: switch (sub) { case 0x01: /* SCOTTISH */ /* old, superseded by LANG_SCOTTISH_GAELIC */ return "gd_GB"; case SUBLANG_IRISH_IRELAND: return "ga_IE"; } return "ga"; case LANG_GALICIAN: switch (sub) { case SUBLANG_GALICIAN_SPAIN: return "gl_ES"; } return "gl"; case LANG_GEORGIAN: switch (sub) { case SUBLANG_GEORGIAN_GEORGIA: return "ka_GE"; } return "ka"; case LANG_GERMAN: switch (sub) { case SUBLANG_GERMAN: return "de_DE"; case SUBLANG_GERMAN_SWISS: return "de_CH"; case SUBLANG_GERMAN_AUSTRIAN: return "de_AT"; case SUBLANG_GERMAN_LUXEMBOURG: return "de_LU"; case SUBLANG_GERMAN_LIECHTENSTEIN: return "de_LI"; } return "de"; case LANG_GREEK: switch (sub) { case SUBLANG_GREEK_GREECE: return "el_GR"; } return "el"; case LANG_GREENLANDIC: switch (sub) { case SUBLANG_GREENLANDIC_GREENLAND: return "kl_GL"; } return "kl"; case LANG_GUARANI: switch (sub) { case SUBLANG_DEFAULT: return "gn_PY"; } return "gn"; case LANG_GUJARATI: switch (sub) { case SUBLANG_GUJARATI_INDIA: return "gu_IN"; } return "gu"; case LANG_HAUSA: switch (sub) { case 0x1f: return "ha"; case SUBLANG_HAUSA_NIGERIA_LATIN: return "ha_NG"; } return "ha"; case LANG_HAWAIIAN: /* FIXME: Do they mean Hawaiian ("haw_US", 1000 speakers) or Hawaii Creole English ("cpe_US", 600000 speakers)? */ switch (sub) { case SUBLANG_DEFAULT: return "cpe_US"; } return "cpe"; case LANG_HEBREW: switch (sub) { case SUBLANG_HEBREW_ISRAEL: return "he_IL"; } return "he"; case LANG_HINDI: switch (sub) { case SUBLANG_HINDI_INDIA: return "hi_IN"; } return "hi"; case LANG_HUNGARIAN: switch (sub) { case SUBLANG_HUNGARIAN_HUNGARY: return "hu_HU"; } return "hu"; case LANG_IBIBIO: switch (sub) { case SUBLANG_DEFAULT: return "nic_NG"; } return "nic"; case LANG_ICELANDIC: switch (sub) { case SUBLANG_ICELANDIC_ICELAND: return "is_IS"; } return "is"; case LANG_IGBO: switch (sub) { case SUBLANG_IGBO_NIGERIA: return "ig_NG"; } return "ig"; case LANG_INDONESIAN: switch (sub) { case SUBLANG_INDONESIAN_INDONESIA: return "id_ID"; } return "id"; case LANG_INUKTITUT: switch (sub) { case 0x1e: return "iu"; /* syllabic */ case SUBLANG_INUKTITUT_CANADA: return "iu_CA"; /* syllabic */ case 0x1f: return "iu@latin"; case SUBLANG_INUKTITUT_CANADA_LATIN: return "iu_CA@latin"; } return "iu"; case LANG_ITALIAN: switch (sub) { case SUBLANG_ITALIAN: return "it_IT"; case SUBLANG_ITALIAN_SWISS: return "it_CH"; } return "it"; case LANG_JAPANESE: switch (sub) { case SUBLANG_JAPANESE_JAPAN: return "ja_JP"; } return "ja"; case LANG_KANNADA: switch (sub) { case SUBLANG_KANNADA_INDIA: return "kn_IN"; } return "kn"; case LANG_KANURI: switch (sub) { case SUBLANG_DEFAULT: return "kr_NG"; } return "kr"; case LANG_KASHMIRI: switch (sub) { case SUBLANG_DEFAULT: return "ks_PK"; case SUBLANG_KASHMIRI_INDIA: return "ks_IN"; } return "ks"; case LANG_KAZAK: switch (sub) { case SUBLANG_KAZAK_KAZAKHSTAN: return "kk_KZ"; } return "kk"; case LANG_KICHE: /* FIXME: Adjust this when such locales appear on Unix. */ switch (sub) { case SUBLANG_KICHE_GUATEMALA: return "qut_GT"; } return "qut"; case LANG_KINYARWANDA: switch (sub) { case SUBLANG_KINYARWANDA_RWANDA: return "rw_RW"; } return "rw"; case LANG_KONKANI: /* FIXME: Adjust this when such locales appear on Unix. */ switch (sub) { case SUBLANG_KONKANI_INDIA: return "kok_IN"; } return "kok"; case LANG_KOREAN: switch (sub) { case SUBLANG_DEFAULT: return "ko_KR"; } return "ko"; case LANG_KYRGYZ: switch (sub) { case SUBLANG_KYRGYZ_KYRGYZSTAN: return "ky_KG"; } return "ky"; case LANG_LAO: switch (sub) { case SUBLANG_LAO_LAOS: return "lo_LA"; } return "lo"; case LANG_LATIN: switch (sub) { case SUBLANG_DEFAULT: return "la_VA"; } return "la"; case LANG_LATVIAN: switch (sub) { case SUBLANG_LATVIAN_LATVIA: return "lv_LV"; } return "lv"; case LANG_LITHUANIAN: switch (sub) { case SUBLANG_LITHUANIAN_LITHUANIA: return "lt_LT"; } return "lt"; case LANG_LUXEMBOURGISH: switch (sub) { case SUBLANG_LUXEMBOURGISH_LUXEMBOURG: return "lb_LU"; } return "lb"; case LANG_MACEDONIAN: switch (sub) { case SUBLANG_MACEDONIAN_MACEDONIA: return "mk_MK"; } return "mk"; case LANG_MALAY: switch (sub) { case SUBLANG_MALAY_MALAYSIA: return "ms_MY"; case SUBLANG_MALAY_BRUNEI_DARUSSALAM: return "ms_BN"; } return "ms"; case LANG_MALAYALAM: switch (sub) { case SUBLANG_MALAYALAM_INDIA: return "ml_IN"; } return "ml"; case LANG_MALTESE: switch (sub) { case SUBLANG_MALTESE_MALTA: return "mt_MT"; } return "mt"; case LANG_MANIPURI: /* FIXME: Adjust this when such locales appear on Unix. */ switch (sub) { case SUBLANG_DEFAULT: return "mni_IN"; } return "mni"; case LANG_MAORI: switch (sub) { case SUBLANG_MAORI_NEW_ZEALAND: return "mi_NZ"; } return "mi"; case LANG_MAPUDUNGUN: switch (sub) { case SUBLANG_MAPUDUNGUN_CHILE: return "arn_CL"; } return "arn"; case LANG_MARATHI: switch (sub) { case SUBLANG_MARATHI_INDIA: return "mr_IN"; } return "mr"; case LANG_MOHAWK: switch (sub) { case SUBLANG_MOHAWK_CANADA: return "moh_CA"; } return "moh"; case LANG_MONGOLIAN: switch (sub) { case SUBLANG_MONGOLIAN_CYRILLIC_MONGOLIA: case 0x1e: return "mn_MN"; case SUBLANG_MONGOLIAN_PRC: case 0x1f: return "mn_CN"; } return "mn"; /* Ambiguous: could be "mn_CN" or "mn_MN". */ case LANG_NEPALI: switch (sub) { case SUBLANG_NEPALI_NEPAL: return "ne_NP"; case SUBLANG_NEPALI_INDIA: return "ne_IN"; } return "ne"; case LANG_NORWEGIAN: switch (sub) { case 0x1f: return "nb"; case SUBLANG_NORWEGIAN_BOKMAL: return "nb_NO"; case 0x1e: return "nn"; case SUBLANG_NORWEGIAN_NYNORSK: return "nn_NO"; } return "no"; case LANG_OCCITAN: switch (sub) { case SUBLANG_OCCITAN_FRANCE: return "oc_FR"; } return "oc"; case LANG_ORIYA: switch (sub) { case SUBLANG_ORIYA_INDIA: return "or_IN"; } return "or"; case LANG_OROMO: switch (sub) { case SUBLANG_DEFAULT: return "om_ET"; } return "om"; case LANG_PAPIAMENTU: switch (sub) { case SUBLANG_DEFAULT: return "pap_AN"; } return "pap"; case LANG_PASHTO: switch (sub) { case SUBLANG_PASHTO_AFGHANISTAN: return "ps_AF"; } return "ps"; /* Ambiguous: could be "ps_PK" or "ps_AF". */ case LANG_POLISH: switch (sub) { case SUBLANG_POLISH_POLAND: return "pl_PL"; } return "pl"; case LANG_PORTUGUESE: switch (sub) { /* Hmm. SUBLANG_PORTUGUESE_BRAZILIAN == SUBLANG_DEFAULT. Same phenomenon as SUBLANG_ENGLISH_US == SUBLANG_DEFAULT. */ case SUBLANG_PORTUGUESE_BRAZILIAN: return "pt_BR"; case SUBLANG_PORTUGUESE: return "pt_PT"; } return "pt"; case LANG_PUNJABI: switch (sub) { case SUBLANG_PUNJABI_INDIA: return "pa_IN"; /* Gurmukhi script */ case SUBLANG_PUNJABI_PAKISTAN: return "pa_PK"; /* Arabic script */ } return "pa"; case LANG_QUECHUA: /* Note: Microsoft uses the non-ISO language code "quz". */ switch (sub) { case SUBLANG_QUECHUA_BOLIVIA: return "qu_BO"; case SUBLANG_QUECHUA_ECUADOR: return "qu_EC"; case SUBLANG_QUECHUA_PERU: return "qu_PE"; } return "qu"; case LANG_ROMANIAN: switch (sub) { case SUBLANG_ROMANIAN_ROMANIA: return "ro_RO"; case SUBLANG_ROMANIAN_MOLDOVA: return "ro_MD"; } return "ro"; case LANG_ROMANSH: switch (sub) { case SUBLANG_ROMANSH_SWITZERLAND: return "rm_CH"; } return "rm"; case LANG_RUSSIAN: switch (sub) { case SUBLANG_RUSSIAN_RUSSIA: return "ru_RU"; case SUBLANG_RUSSIAN_MOLDAVIA: return "ru_MD"; } return "ru"; /* Ambiguous: could be "ru_RU" or "ru_UA" or "ru_MD". */ case LANG_SAMI: switch (sub) { /* Northern Sami */ case 0x00: return "se"; case SUBLANG_SAMI_NORTHERN_NORWAY: return "se_NO"; case SUBLANG_SAMI_NORTHERN_SWEDEN: return "se_SE"; case SUBLANG_SAMI_NORTHERN_FINLAND: return "se_FI"; /* Lule Sami */ case 0x1f: return "smj"; case SUBLANG_SAMI_LULE_NORWAY: return "smj_NO"; case SUBLANG_SAMI_LULE_SWEDEN: return "smj_SE"; /* Southern Sami */ case 0x1e: return "sma"; case SUBLANG_SAMI_SOUTHERN_NORWAY: return "sma_NO"; case SUBLANG_SAMI_SOUTHERN_SWEDEN: return "sma_SE"; /* Skolt Sami */ case 0x1d: return "sms"; case SUBLANG_SAMI_SKOLT_FINLAND: return "sms_FI"; /* Inari Sami */ case 0x1c: return "smn"; case SUBLANG_SAMI_INARI_FINLAND: return "smn_FI"; } return "se"; /* or "smi"? */ case LANG_SANSKRIT: switch (sub) { case SUBLANG_SANSKRIT_INDIA: return "sa_IN"; } return "sa"; case LANG_SCOTTISH_GAELIC: switch (sub) { case SUBLANG_DEFAULT: return "gd_GB"; } return "gd"; case LANG_SINDHI: switch (sub) { case SUBLANG_SINDHI_INDIA: return "sd_IN"; case SUBLANG_SINDHI_PAKISTAN: return "sd_PK"; /*case SUBLANG_SINDHI_AFGHANISTAN: return "sd_AF";*/ } return "sd"; case LANG_SINHALESE: switch (sub) { case SUBLANG_SINHALESE_SRI_LANKA: return "si_LK"; } return "si"; case LANG_SLOVAK: switch (sub) { case SUBLANG_SLOVAK_SLOVAKIA: return "sk_SK"; } return "sk"; case LANG_SLOVENIAN: switch (sub) { case SUBLANG_SLOVENIAN_SLOVENIA: return "sl_SI"; } return "sl"; case LANG_SOMALI: switch (sub) { case SUBLANG_DEFAULT: return "so_SO"; } return "so"; case LANG_SORBIAN: /* FIXME: Adjust this when such locales appear on Unix. */ switch (sub) { /* Upper Sorbian */ case 0x00: return "hsb"; case SUBLANG_UPPER_SORBIAN_GERMANY: return "hsb_DE"; /* Lower Sorbian */ case 0x1f: return "dsb"; case SUBLANG_LOWER_SORBIAN_GERMANY: return "dsb_DE"; } return "wen"; case LANG_SOTHO: /* calls it "Sepedi"; according to it's the same as Northern Sotho. */ switch (sub) { case SUBLANG_SOTHO_SOUTH_AFRICA: return "nso_ZA"; } return "nso"; case LANG_SPANISH: switch (sub) { case SUBLANG_SPANISH: return "es_ES"; case SUBLANG_SPANISH_MEXICAN: return "es_MX"; case SUBLANG_SPANISH_MODERN: return "es_ES@modern"; /* not seen on Unix */ case SUBLANG_SPANISH_GUATEMALA: return "es_GT"; case SUBLANG_SPANISH_COSTA_RICA: return "es_CR"; case SUBLANG_SPANISH_PANAMA: return "es_PA"; case SUBLANG_SPANISH_DOMINICAN_REPUBLIC: return "es_DO"; case SUBLANG_SPANISH_VENEZUELA: return "es_VE"; case SUBLANG_SPANISH_COLOMBIA: return "es_CO"; case SUBLANG_SPANISH_PERU: return "es_PE"; case SUBLANG_SPANISH_ARGENTINA: return "es_AR"; case SUBLANG_SPANISH_ECUADOR: return "es_EC"; case SUBLANG_SPANISH_CHILE: return "es_CL"; case SUBLANG_SPANISH_URUGUAY: return "es_UY"; case SUBLANG_SPANISH_PARAGUAY: return "es_PY"; case SUBLANG_SPANISH_BOLIVIA: return "es_BO"; case SUBLANG_SPANISH_EL_SALVADOR: return "es_SV"; case SUBLANG_SPANISH_HONDURAS: return "es_HN"; case SUBLANG_SPANISH_NICARAGUA: return "es_NI"; case SUBLANG_SPANISH_PUERTO_RICO: return "es_PR"; case SUBLANG_SPANISH_US: return "es_US"; } return "es"; case LANG_SUTU: switch (sub) { case SUBLANG_DEFAULT: return "bnt_TZ"; /* or "st_LS" or "nso_ZA"? */ } return "bnt"; case LANG_SWAHILI: switch (sub) { case SUBLANG_SWAHILI_KENYA: return "sw_KE"; } return "sw"; case LANG_SWEDISH: switch (sub) { case SUBLANG_SWEDISH_SWEDEN: return "sv_SE"; case SUBLANG_SWEDISH_FINLAND: return "sv_FI"; } return "sv"; case LANG_SYRIAC: switch (sub) { case SUBLANG_SYRIAC_SYRIA: return "syr_SY"; /* An extinct language. */ } return "syr"; case LANG_TAGALOG: switch (sub) { case SUBLANG_TAGALOG_PHILIPPINES: return "tl_PH"; /* or "fil_PH"? */ } return "tl"; /* or "fil"? */ case LANG_TAJIK: switch (sub) { case 0x1f: return "tg"; case SUBLANG_TAJIK_TAJIKISTAN: return "tg_TJ"; } return "tg"; case LANG_TAMAZIGHT: /* Note: Microsoft uses the non-ISO language code "tmz". */ switch (sub) { /* FIXME: Adjust this when Tamazight locales appear on Unix. */ case SUBLANG_TAMAZIGHT_ARABIC: return "ber_MA@arabic"; case 0x1f: return "ber@latin"; case SUBLANG_TAMAZIGHT_ALGERIA_LATIN: return "ber_DZ@latin"; } return "ber"; case LANG_TAMIL: switch (sub) { case SUBLANG_TAMIL_INDIA: return "ta_IN"; } return "ta"; /* Ambiguous: could be "ta_IN" or "ta_LK" or "ta_SG". */ case LANG_TATAR: switch (sub) { case SUBLANG_TATAR_RUSSIA: return "tt_RU"; } return "tt"; case LANG_TELUGU: switch (sub) { case SUBLANG_TELUGU_INDIA: return "te_IN"; } return "te"; case LANG_THAI: switch (sub) { case SUBLANG_THAI_THAILAND: return "th_TH"; } return "th"; case LANG_TIBETAN: switch (sub) { case SUBLANG_TIBETAN_PRC: /* Most Tibetans would not like "bo_CN". But Tibet does not yet have a country code of its own. */ return "bo"; case SUBLANG_TIBETAN_BHUTAN: return "bo_BT"; } return "bo"; case LANG_TIGRINYA: switch (sub) { case SUBLANG_TIGRINYA_ETHIOPIA: return "ti_ET"; case SUBLANG_TIGRINYA_ERITREA: return "ti_ER"; } return "ti"; case LANG_TSONGA: switch (sub) { case SUBLANG_DEFAULT: return "ts_ZA"; } return "ts"; case LANG_TSWANA: /* Spoken in South Africa, Botswana. */ switch (sub) { case SUBLANG_TSWANA_SOUTH_AFRICA: return "tn_ZA"; } return "tn"; case LANG_TURKISH: switch (sub) { case SUBLANG_TURKISH_TURKEY: return "tr_TR"; } return "tr"; case LANG_TURKMEN: switch (sub) { case SUBLANG_TURKMEN_TURKMENISTAN: return "tk_TM"; } return "tk"; case LANG_UIGHUR: switch (sub) { case SUBLANG_UIGHUR_PRC: return "ug_CN"; } return "ug"; case LANG_UKRAINIAN: switch (sub) { case SUBLANG_UKRAINIAN_UKRAINE: return "uk_UA"; } return "uk"; case LANG_URDU: switch (sub) { case SUBLANG_URDU_PAKISTAN: return "ur_PK"; case SUBLANG_URDU_INDIA: return "ur_IN"; } return "ur"; case LANG_UZBEK: switch (sub) { case 0x1f: return "uz"; case SUBLANG_UZBEK_LATIN: return "uz_UZ"; case 0x1e: return "uz@cyrillic"; case SUBLANG_UZBEK_CYRILLIC: return "uz_UZ@cyrillic"; } return "uz"; case LANG_VENDA: switch (sub) { case SUBLANG_DEFAULT: return "ve_ZA"; } return "ve"; case LANG_VIETNAMESE: switch (sub) { case SUBLANG_VIETNAMESE_VIETNAM: return "vi_VN"; } return "vi"; case LANG_WELSH: switch (sub) { case SUBLANG_WELSH_UNITED_KINGDOM: return "cy_GB"; } return "cy"; case LANG_WOLOF: switch (sub) { case SUBLANG_WOLOF_SENEGAL: return "wo_SN"; } return "wo"; case LANG_XHOSA: switch (sub) { case SUBLANG_XHOSA_SOUTH_AFRICA: return "xh_ZA"; } return "xh"; case LANG_YAKUT: switch (sub) { case SUBLANG_YAKUT_RUSSIA: return "sah_RU"; } return "sah"; case LANG_YI: switch (sub) { case SUBLANG_YI_PRC: return "ii_CN"; } return "ii"; case LANG_YIDDISH: switch (sub) { case SUBLANG_DEFAULT: return "yi_IL"; } return "yi"; case LANG_YORUBA: switch (sub) { case SUBLANG_YORUBA_NIGERIA: return "yo_NG"; } return "yo"; case LANG_ZULU: switch (sub) { case SUBLANG_ZULU_SOUTH_AFRICA: return "zu_ZA"; } return "zu"; default: return "C"; } } } # if !defined IN_LIBINTL static # endif const char * gl_locale_name_from_win32_LCID (LCID lcid) { LANGID langid; /* Strip off the sorting rules, keep only the language part. */ langid = LANGIDFROMLCID (lcid); return gl_locale_name_from_win32_LANGID (langid); } # ifdef WINDOWS_NATIVE /* Two variables to interface between get_lcid and the EnumLocales callback function below. */ static LCID found_lcid; static char lname[LC_MAX * (LOCALE_NAME_MAX_LENGTH + 1) + 1]; /* Callback function for EnumLocales. */ static BOOL CALLBACK enum_locales_fn (LPTSTR locale_num_str) { char *endp; char locval[2 * LOCALE_NAME_MAX_LENGTH + 1 + 1]; LCID try_lcid = strtoul (locale_num_str, &endp, 16); if (GetLocaleInfo (try_lcid, LOCALE_SENGLANGUAGE, locval, LOCALE_NAME_MAX_LENGTH)) { strcat (locval, "_"); if (GetLocaleInfo (try_lcid, LOCALE_SENGCOUNTRY, locval + strlen (locval), LOCALE_NAME_MAX_LENGTH)) { size_t locval_len = strlen (locval); if (strncmp (locval, lname, locval_len) == 0 && (lname[locval_len] == '.' || lname[locval_len] == '\0')) { found_lcid = try_lcid; return FALSE; } } } return TRUE; } /* This lock protects the get_lcid against multiple simultaneous calls. */ gl_lock_define_initialized(static, get_lcid_lock) /* Return the Locale ID (LCID) number given the locale's name, a string, in LOCALE_NAME. This works by enumerating all the locales supported by the system, until we find one whose name matches LOCALE_NAME. */ static LCID get_lcid (const char *locale_name) { /* A simple cache. */ static LCID last_lcid; static char last_locale[1000]; /* Lock while looking for an LCID, to protect access to static variables: last_lcid, last_locale, found_lcid, and lname. */ gl_lock_lock (get_lcid_lock); if (last_lcid > 0 && strcmp (locale_name, last_locale) == 0) { gl_lock_unlock (get_lcid_lock); return last_lcid; } strncpy (lname, locale_name, sizeof (lname) - 1); lname[sizeof (lname) - 1] = '\0'; found_lcid = 0; EnumSystemLocales (enum_locales_fn, LCID_SUPPORTED); if (found_lcid > 0) { last_lcid = found_lcid; strcpy (last_locale, locale_name); } gl_lock_unlock (get_lcid_lock); return found_lcid; } # endif #endif #if HAVE_USELOCALE /* glibc, Solaris >= 12 or Mac OS X */ /* Simple hash set of strings. We don't want to drag in lots of hash table code here. */ # define SIZE_BITS (sizeof (size_t) * CHAR_BIT) /* A hash function for NUL-terminated char* strings using the method described by Bruno Haible. See http://www.haible.de/bruno/hashfunc.html. */ static size_t _GL_ATTRIBUTE_PURE string_hash (const void *x) { const char *s = (const char *) x; size_t h = 0; for (; *s; s++) h = *s + ((h << 9) | (h >> (SIZE_BITS - 9))); return h; } /* A hash table of fixed size. Multiple threads can access it read-only simultaneously, but only one thread can insert into it at the same time. */ /* A node in a hash bucket collision list. */ struct hash_node { struct hash_node * volatile next; char contents[FLEXIBLE_ARRAY_MEMBER]; }; # define HASH_TABLE_SIZE 257 static struct hash_node * volatile struniq_hash_table[HASH_TABLE_SIZE] /* = { NULL, ..., NULL } */; /* This lock protects the struniq_hash_table against multiple simultaneous insertions. */ gl_lock_define_initialized(static, struniq_lock) /* Store a copy of the given string in a string pool with indefinite extent. Return a pointer to this copy. */ static const char * struniq (const char *string) { size_t hashcode = string_hash (string); size_t slot = hashcode % HASH_TABLE_SIZE; size_t size; struct hash_node *new_node; struct hash_node *p; for (p = struniq_hash_table[slot]; p != NULL; p = p->next) if (strcmp (p->contents, string) == 0) return p->contents; size = strlen (string) + 1; new_node = (struct hash_node *) malloc (FLEXSIZEOF (struct hash_node, contents, size)); if (new_node == NULL) /* Out of memory. Return a statically allocated string. */ return "C"; memcpy (new_node->contents, string, size); /* Lock while inserting new_node. */ gl_lock_lock (struniq_lock); /* Check whether another thread already added the string while we were waiting on the lock. */ for (p = struniq_hash_table[slot]; p != NULL; p = p->next) if (strcmp (p->contents, string) == 0) { free (new_node); new_node = p; goto done; } /* Really insert new_node into the hash table. Fill new_node entirely first, because other threads may be iterating over the linked list. */ new_node->next = struniq_hash_table[slot]; struniq_hash_table[slot] = new_node; done: /* Unlock after new_node is inserted. */ gl_lock_unlock (struniq_lock); return new_node->contents; } #endif #if defined IN_LIBINTL || HAVE_USELOCALE /* Like gl_locale_name_thread, except that the result is not in storage of indefinite extent. */ # if !defined IN_LIBINTL static # endif const char * gl_locale_name_thread_unsafe (int category, const char *categoryname) { # if HAVE_USELOCALE { locale_t thread_locale = uselocale (NULL); if (thread_locale != LC_GLOBAL_LOCALE) { # if __GLIBC__ >= 2 && !defined __UCLIBC__ /* Work around an incorrect definition of the _NL_LOCALE_NAME macro in glibc < 2.12. See . */ const char *name = nl_langinfo (_NL_ITEM ((category), _NL_ITEM_INDEX (-1))); if (name[0] == '\0') /* Fallback code for glibc < 2.4, which did not implement nl_langinfo (_NL_LOCALE_NAME (category)). */ name = thread_locale->__names[category]; return name; # elif defined __FreeBSD__ || (defined __APPLE__ && defined __MACH__) /* FreeBSD, Mac OS X */ int mask; switch (category) { case LC_CTYPE: mask = LC_CTYPE_MASK; break; case LC_NUMERIC: mask = LC_NUMERIC_MASK; break; case LC_TIME: mask = LC_TIME_MASK; break; case LC_COLLATE: mask = LC_COLLATE_MASK; break; case LC_MONETARY: mask = LC_MONETARY_MASK; break; case LC_MESSAGES: mask = LC_MESSAGES_MASK; break; default: /* We shouldn't get here. */ return ""; } return querylocale (mask, thread_locale); # elif defined __sun && HAVE_GETLOCALENAME_L /* Solaris >= 12. */ return getlocalename_l (category, thread_locale); # elif defined __ANDROID__ return MB_CUR_MAX == 4 ? "C.UTF-8" : "C"; # endif } } # endif return NULL; } #endif const char * gl_locale_name_thread (int category, const char *categoryname) { #if HAVE_USELOCALE const char *name = gl_locale_name_thread_unsafe (category, categoryname); if (name != NULL) return struniq (name); #elif defined WINDOWS_NATIVE if (LC_MIN <= category && category <= LC_MAX) { char *locname = setlocale (category, NULL); LCID lcid = 0; /* If CATEGORY is LC_ALL, the result might be a semi-colon separated list of locales. We need only one, so we take the one corresponding to LC_CTYPE, as the most important for character translations. */ if (strchr (locname, ';')) locname = setlocale (LC_CTYPE, NULL); /* Convert locale name to LCID. We don't want to use LocaleNameToLCID because (a) it is only available since Vista, and (b) it doesn't accept locale names returned by 'setlocale'. */ lcid = get_lcid (locname); if (lcid > 0) return gl_locale_name_from_win32_LCID (lcid); } #endif return NULL; } /* XPG3 defines the result of 'setlocale (category, NULL)' as: "Directs 'setlocale()' to query 'category' and return the current setting of 'local'." However it does not specify the exact format. Neither do SUSV2 and ISO C 99. So we can use this feature only on selected systems (e.g. those using GNU C Library). */ #if defined _LIBC || ((defined __GLIBC__ && __GLIBC__ >= 2) && !defined __UCLIBC__) # define HAVE_LOCALE_NULL #endif const char * gl_locale_name_posix (int category, const char *categoryname) { /* Use the POSIX methods of looking to 'LC_ALL', 'LC_xxx', and 'LANG'. On some systems this can be done by the 'setlocale' function itself. */ #if defined HAVE_SETLOCALE && defined HAVE_LC_MESSAGES && defined HAVE_LOCALE_NULL return setlocale (category, NULL); #else /* On other systems we ignore what setlocale reports and instead look at the environment variables directly. This is necessary 1. on systems which have a facility for customizing the default locale (Mac OS X, native Windows, Cygwin) and where the system's setlocale() function ignores this default locale (Mac OS X, Cygwin), in two cases: a. when the user missed to use the setlocale() override from libintl (for example by not including ), b. when setlocale supports only the "C" locale, such as on Cygwin 1.5.x. In this case even the override from libintl cannot help. 2. on all systems where setlocale supports only the "C" locale. */ /* Strictly speaking, it is a POSIX violation to look at the environment variables regardless whether setlocale has been called or not. POSIX says: "For C-language programs, the POSIX locale shall be the default locale when the setlocale() function is not called." But we assume that all programs that use internationalized APIs call setlocale (LC_ALL, ""). */ return gl_locale_name_environ (category, categoryname); #endif } const char * gl_locale_name_environ (int category, const char *categoryname) { const char *retval; /* Setting of LC_ALL overrides all other. */ retval = getenv ("LC_ALL"); if (retval != NULL && retval[0] != '\0') return retval; /* Next comes the name of the desired category. */ retval = getenv (categoryname); if (retval != NULL && retval[0] != '\0') return retval; /* Last possibility is the LANG environment variable. */ retval = getenv ("LANG"); if (retval != NULL && retval[0] != '\0') { #if HAVE_CFLOCALECOPYCURRENT || HAVE_CFPREFERENCESCOPYAPPVALUE /* Mac OS X 10.2 or newer. Ignore invalid LANG value set by the Terminal application. */ if (strcmp (retval, "UTF-8") != 0) #endif #if defined __CYGWIN__ /* Cygwin. Ignore dummy LANG value set by ~/.profile. */ if (strcmp (retval, "C.UTF-8") != 0) #endif return retval; } return NULL; } const char * gl_locale_name_default (void) { /* POSIX:2001 says: "All implementations shall define a locale as the default locale, to be invoked when no environment variables are set, or set to the empty string. This default locale can be the POSIX locale or any other implementation-defined locale. Some implementations may provide facilities for local installation administrators to set the default locale, customizing it for each location. POSIX:2001 does not require such a facility. The systems with such a facility are Mac OS X and Windows: They provide a GUI that allows the user to choose a locale. - On Mac OS X, by default, none of LC_* or LANG are set. Starting with Mac OS X 10.4 or 10.5, LANG is set for processes launched by the 'Terminal' application (but sometimes to an incorrect value "UTF-8"). When no environment variable is set, setlocale (LC_ALL, "") uses the "C" locale. - On native Windows, by default, none of LC_* or LANG are set. When no environment variable is set, setlocale (LC_ALL, "") uses the locale chosen by the user. - On Cygwin 1.5.x, by default, none of LC_* or LANG are set. When no environment variable is set, setlocale (LC_ALL, "") uses the "C" locale. - On Cygwin 1.7, by default, LANG is set to "C.UTF-8" when the default ~/.profile is executed. When no environment variable is set, setlocale (LC_ALL, "") uses the "C.UTF-8" locale, which operates in the same way as the "C" locale. */ #if !(HAVE_CFLOCALECOPYCURRENT || HAVE_CFPREFERENCESCOPYAPPVALUE || defined WINDOWS_NATIVE || defined __CYGWIN__) /* The system does not have a way of setting the locale, other than the POSIX specified environment variables. We use C as default locale. */ return "C"; #else /* Return an XPG style locale name language[_territory][@modifier]. Don't even bother determining the codeset; it's not useful in this context, because message catalogs are not specific to a single codeset. */ # if HAVE_CFLOCALECOPYCURRENT || HAVE_CFPREFERENCESCOPYAPPVALUE /* Mac OS X 10.2 or newer */ { /* Cache the locale name, since CoreFoundation calls are expensive. */ static const char *cached_localename; if (cached_localename == NULL) { char namebuf[256]; # if HAVE_CFLOCALECOPYCURRENT /* Mac OS X 10.3 or newer */ CFLocaleRef locale = CFLocaleCopyCurrent (); CFStringRef name = CFLocaleGetIdentifier (locale); if (CFStringGetCString (name, namebuf, sizeof (namebuf), kCFStringEncodingASCII)) { gl_locale_name_canonicalize (namebuf); cached_localename = strdup (namebuf); } CFRelease (locale); # elif HAVE_CFPREFERENCESCOPYAPPVALUE /* Mac OS X 10.2 or newer */ CFTypeRef value = CFPreferencesCopyAppValue (CFSTR ("AppleLocale"), kCFPreferencesCurrentApplication); if (value != NULL && CFGetTypeID (value) == CFStringGetTypeID () && CFStringGetCString ((CFStringRef)value, namebuf, sizeof (namebuf), kCFStringEncodingASCII)) { gl_locale_name_canonicalize (namebuf); cached_localename = strdup (namebuf); } # endif if (cached_localename == NULL) cached_localename = "C"; } return cached_localename; } # endif # if defined WINDOWS_NATIVE || defined __CYGWIN__ /* Native Windows or Cygwin */ { LCID lcid; /* Use native Windows API locale ID. */ lcid = GetThreadLocale (); return gl_locale_name_from_win32_LCID (lcid); } # endif #endif } /* Determine the current locale's name, and canonicalize it into XPG syntax language[_territory][.codeset][@modifier] The codeset part in the result is not reliable; the locale_charset() should be used for codeset information instead. The result must not be freed; it is statically allocated. */ const char * gl_locale_name (int category, const char *categoryname) { const char *retval; retval = gl_locale_name_thread (category, categoryname); if (retval != NULL) return retval; retval = gl_locale_name_posix (category, categoryname); if (retval != NULL) return retval; return gl_locale_name_default (); } gnuastro-0.2.33-8a3b/bootstrapped/tests/fd-hook.c0000644000175000017500000000701213004436755016467 00000000000000/* Hook for making making file descriptor functions close(), ioctl() extensible. Copyright (C) 2009-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2009. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include "fd-hook.h" #include /* Currently, this entire code is only needed for the handling of sockets on native Windows platforms. */ #if WINDOWS_SOCKETS /* The first and last link in the doubly linked list. Initially the list is empty. */ static struct fd_hook anchor = { &anchor, &anchor, NULL, NULL }; int execute_close_hooks (const struct fd_hook *remaining_list, gl_close_fn primary, int fd) { if (remaining_list == &anchor) /* End of list reached. */ return primary (fd); else return remaining_list->private_close_fn (remaining_list->private_next, primary, fd); } int execute_all_close_hooks (gl_close_fn primary, int fd) { return execute_close_hooks (anchor.private_next, primary, fd); } int execute_ioctl_hooks (const struct fd_hook *remaining_list, gl_ioctl_fn primary, int fd, int request, void *arg) { if (remaining_list == &anchor) /* End of list reached. */ return primary (fd, request, arg); else return remaining_list->private_ioctl_fn (remaining_list->private_next, primary, fd, request, arg); } int execute_all_ioctl_hooks (gl_ioctl_fn primary, int fd, int request, void *arg) { return execute_ioctl_hooks (anchor.private_next, primary, fd, request, arg); } void register_fd_hook (close_hook_fn close_hook, ioctl_hook_fn ioctl_hook, struct fd_hook *link) { if (close_hook == NULL) close_hook = execute_close_hooks; if (ioctl_hook == NULL) ioctl_hook = execute_ioctl_hooks; if (link->private_next == NULL && link->private_prev == NULL) { /* Add the link to the doubly linked list. */ link->private_next = anchor.private_next; link->private_prev = &anchor; link->private_close_fn = close_hook; link->private_ioctl_fn = ioctl_hook; anchor.private_next->private_prev = link; anchor.private_next = link; } else { /* The link is already in use. */ if (link->private_close_fn != close_hook || link->private_ioctl_fn != ioctl_hook) abort (); } } void unregister_fd_hook (struct fd_hook *link) { struct fd_hook *next = link->private_next; struct fd_hook *prev = link->private_prev; if (next != NULL && prev != NULL) { /* The link is in use. Remove it from the doubly linked list. */ prev->private_next = next; next->private_prev = prev; /* Clear the link, to mark it unused. */ link->private_next = NULL; link->private_prev = NULL; link->private_close_fn = NULL; link->private_ioctl_fn = NULL; } } #endif gnuastro-0.2.33-8a3b/bootstrapped/tests/c-strncasecmp.c0000644000175000017500000000310613004436755017702 00000000000000/* c-strncasecmp.c -- case insensitive string comparator in C locale Copyright (C) 1998-1999, 2005-2006, 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include "c-strcase.h" #include #include "c-ctype.h" int c_strncasecmp (const char *s1, const char *s2, size_t n) { register const unsigned char *p1 = (const unsigned char *) s1; register const unsigned char *p2 = (const unsigned char *) s2; unsigned char c1, c2; if (p1 == p2 || n == 0) return 0; do { c1 = c_tolower (*p1); c2 = c_tolower (*p2); if (--n == 0 || c1 == '\0') break; ++p1; ++p2; } while (c1 == c2); if (UCHAR_MAX <= INT_MAX) return c1 - c2; else /* On machines where 'char' and 'int' are types of the same size, the difference of two 'unsigned char' values - including the sign bit - doesn't fit in an 'int'. */ return (c1 > c2 ? 1 : c1 < c2 ? -1 : 0); } gnuastro-0.2.33-8a3b/bootstrapped/tests/c-strcasecmp.c0000644000175000017500000000304413004436755017525 00000000000000/* c-strcasecmp.c -- case insensitive string comparator in C locale Copyright (C) 1998-1999, 2005-2006, 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include "c-strcase.h" #include #include "c-ctype.h" int c_strcasecmp (const char *s1, const char *s2) { register const unsigned char *p1 = (const unsigned char *) s1; register const unsigned char *p2 = (const unsigned char *) s2; unsigned char c1, c2; if (p1 == p2) return 0; do { c1 = c_tolower (*p1); c2 = c_tolower (*p2); if (c1 == '\0') break; ++p1; ++p2; } while (c1 == c2); if (UCHAR_MAX <= INT_MAX) return c1 - c2; else /* On machines where 'char' and 'int' are types of the same size, the difference of two 'unsigned char' values - including the sign bit - doesn't fit in an 'int'. */ return (c1 > c2 ? 1 : c1 < c2 ? -1 : 0); } gnuastro-0.2.33-8a3b/bootstrapped/tests/c-strcase.h0000644000175000017500000000401413004436755017030 00000000000000/* Case-insensitive string comparison functions in C locale. Copyright (C) 1995-1996, 2001, 2003, 2005, 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef C_STRCASE_H #define C_STRCASE_H #include /* The functions defined in this file assume the "C" locale and a character set without diacritics (ASCII-US or EBCDIC-US or something like that). Even if the "C" locale on a particular system is an extension of the ASCII character set (like on BeOS, where it is UTF-8, or on AmigaOS, where it is ISO-8859-1), the functions in this file recognize only the ASCII characters. More precisely, one of the string arguments must be an ASCII string; the other one can also contain non-ASCII characters (but then the comparison result will be nonzero). */ #ifdef __cplusplus extern "C" { #endif /* Compare strings S1 and S2, ignoring case, returning less than, equal to or greater than zero if S1 is lexicographically less than, equal to or greater than S2. */ extern int c_strcasecmp (const char *s1, const char *s2) _GL_ATTRIBUTE_PURE; /* Compare no more than N characters of strings S1 and S2, ignoring case, returning less than, equal to or greater than zero if S1 is lexicographically less than, equal to or greater than S2. */ extern int c_strncasecmp (const char *s1, const char *s2, size_t n) _GL_ATTRIBUTE_PURE; #ifdef __cplusplus } #endif #endif /* C_STRCASE_H */ gnuastro-0.2.33-8a3b/bootstrapped/tests/binary-io.c0000644000175000017500000000015113004436755017026 00000000000000#include #define BINARY_IO_INLINE _GL_EXTERN_INLINE #include "binary-io.h" typedef int dummy; gnuastro-0.2.33-8a3b/bootstrapped/tests/binary-io.h0000644000175000017500000000472413004436755017045 00000000000000/* Binary mode I/O. Copyright (C) 2001, 2003, 2005, 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _BINARY_H #define _BINARY_H /* For systems that distinguish between text and binary I/O. O_BINARY is guaranteed by the gnulib . */ #include /* The MSVC7 doesn't like to be included after '#define fileno ...', so we include it here first. */ #include #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef BINARY_IO_INLINE # define BINARY_IO_INLINE _GL_INLINE #endif /* set_binary_mode (fd, mode) sets the binary/text I/O mode of file descriptor fd to the given mode (must be O_BINARY or O_TEXT) and returns the previous mode. */ #if O_BINARY # if defined __EMX__ || defined __DJGPP__ || defined __CYGWIN__ # include /* declares setmode() */ # define set_binary_mode setmode # else # define set_binary_mode _setmode # undef fileno # define fileno _fileno # endif #else /* On reasonable systems, binary I/O is the only choice. */ /* Use a function rather than a macro, to avoid gcc warnings "warning: statement with no effect". */ BINARY_IO_INLINE int set_binary_mode (int fd, int mode) { (void) fd; (void) mode; return O_BINARY; } #endif /* SET_BINARY (fd); changes the file descriptor fd to perform binary I/O. */ #if defined __DJGPP__ || defined __EMX__ # include /* declares isatty() */ /* Avoid putting stdin/stdout in binary mode if it is connected to the console, because that would make it impossible for the user to interrupt the program through Ctrl-C or Ctrl-Break. */ # define SET_BINARY(fd) ((void) (!isatty (fd) ? (set_binary_mode (fd, O_BINARY), 0) : 0)) #else # define SET_BINARY(fd) ((void) set_binary_mode (fd, O_BINARY)) #endif _GL_INLINE_HEADER_END #endif /* _BINARY_H */ gnuastro-0.2.33-8a3b/bootstrapped/tests/Makefile.in0000644000175000017500000053252013004464627017047 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY, to the extent permitted by law; without # even the implied warranty of MERCHANTABILITY or FITNESS FOR A # PARTICULAR PURPOSE. @SET_MAKE@ # Copyright (C) 2002-2016 Free Software Foundation, Inc. # # This file is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This file is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this file. If not, see . # # As a special exception to the GNU General Public License, # this file may be distributed as part of a program that # contains a configuration script generated by Autoconf, under # the same distribution terms as the rest of that program. # # Generated by gnulib-tool. 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@GNULIB_COSF@ GNULIB_COSHF = @GNULIB_COSHF@ GNULIB_COSL = @GNULIB_COSL@ GNULIB_DPRINTF = @GNULIB_DPRINTF@ GNULIB_DUP = @GNULIB_DUP@ GNULIB_DUP2 = @GNULIB_DUP2@ GNULIB_DUP3 = @GNULIB_DUP3@ GNULIB_DUPLOCALE = @GNULIB_DUPLOCALE@ GNULIB_ENVIRON = @GNULIB_ENVIRON@ GNULIB_EUIDACCESS = @GNULIB_EUIDACCESS@ GNULIB_EXP2 = @GNULIB_EXP2@ GNULIB_EXP2F = @GNULIB_EXP2F@ GNULIB_EXP2L = @GNULIB_EXP2L@ GNULIB_EXPF = @GNULIB_EXPF@ GNULIB_EXPL = @GNULIB_EXPL@ GNULIB_EXPM1 = @GNULIB_EXPM1@ GNULIB_EXPM1F = @GNULIB_EXPM1F@ GNULIB_EXPM1L = @GNULIB_EXPM1L@ GNULIB_FABSF = @GNULIB_FABSF@ GNULIB_FABSL = @GNULIB_FABSL@ GNULIB_FACCESSAT = @GNULIB_FACCESSAT@ GNULIB_FCHDIR = @GNULIB_FCHDIR@ GNULIB_FCHMODAT = @GNULIB_FCHMODAT@ GNULIB_FCHOWNAT = @GNULIB_FCHOWNAT@ GNULIB_FCLOSE = @GNULIB_FCLOSE@ GNULIB_FCNTL = @GNULIB_FCNTL@ GNULIB_FDATASYNC = @GNULIB_FDATASYNC@ GNULIB_FDOPEN = @GNULIB_FDOPEN@ GNULIB_FFLUSH = @GNULIB_FFLUSH@ GNULIB_FFS = @GNULIB_FFS@ GNULIB_FFSL = @GNULIB_FFSL@ GNULIB_FFSLL = @GNULIB_FFSLL@ GNULIB_FGETC = @GNULIB_FGETC@ GNULIB_FGETS = @GNULIB_FGETS@ GNULIB_FLOOR = @GNULIB_FLOOR@ GNULIB_FLOORF = @GNULIB_FLOORF@ GNULIB_FLOORL = @GNULIB_FLOORL@ GNULIB_FMA = @GNULIB_FMA@ GNULIB_FMAF = @GNULIB_FMAF@ GNULIB_FMAL = @GNULIB_FMAL@ GNULIB_FMOD = @GNULIB_FMOD@ GNULIB_FMODF = @GNULIB_FMODF@ GNULIB_FMODL = @GNULIB_FMODL@ GNULIB_FOPEN = @GNULIB_FOPEN@ GNULIB_FPRINTF = @GNULIB_FPRINTF@ GNULIB_FPRINTF_POSIX = @GNULIB_FPRINTF_POSIX@ GNULIB_FPURGE = @GNULIB_FPURGE@ GNULIB_FPUTC = @GNULIB_FPUTC@ GNULIB_FPUTS = @GNULIB_FPUTS@ GNULIB_FREAD = @GNULIB_FREAD@ GNULIB_FREOPEN = @GNULIB_FREOPEN@ GNULIB_FREXP = @GNULIB_FREXP@ GNULIB_FREXPF = @GNULIB_FREXPF@ GNULIB_FREXPL = @GNULIB_FREXPL@ GNULIB_FSCANF = @GNULIB_FSCANF@ GNULIB_FSEEK = @GNULIB_FSEEK@ GNULIB_FSEEKO = @GNULIB_FSEEKO@ GNULIB_FSTAT = @GNULIB_FSTAT@ GNULIB_FSTATAT = @GNULIB_FSTATAT@ GNULIB_FSYNC = @GNULIB_FSYNC@ GNULIB_FTELL = @GNULIB_FTELL@ GNULIB_FTELLO = @GNULIB_FTELLO@ GNULIB_FTRUNCATE = @GNULIB_FTRUNCATE@ GNULIB_FUTIMENS = @GNULIB_FUTIMENS@ GNULIB_FWRITE = @GNULIB_FWRITE@ GNULIB_GETC = @GNULIB_GETC@ GNULIB_GETCHAR = @GNULIB_GETCHAR@ GNULIB_GETCWD = @GNULIB_GETCWD@ GNULIB_GETDELIM = @GNULIB_GETDELIM@ GNULIB_GETDOMAINNAME = @GNULIB_GETDOMAINNAME@ GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ REPLACE_READ = @REPLACE_READ@ REPLACE_READLINK = @REPLACE_READLINK@ REPLACE_READLINKAT = @REPLACE_READLINKAT@ REPLACE_REALLOC = @REPLACE_REALLOC@ REPLACE_REALPATH = @REPLACE_REALPATH@ REPLACE_REMAINDER = @REPLACE_REMAINDER@ REPLACE_REMAINDERF = @REPLACE_REMAINDERF@ REPLACE_REMAINDERL = @REPLACE_REMAINDERL@ REPLACE_REMOVE = @REPLACE_REMOVE@ REPLACE_RENAME = @REPLACE_RENAME@ REPLACE_RENAMEAT = @REPLACE_RENAMEAT@ REPLACE_RMDIR = @REPLACE_RMDIR@ REPLACE_ROUND = @REPLACE_ROUND@ REPLACE_ROUNDF = @REPLACE_ROUNDF@ 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TESTS_ENVIRONMENT = EXEEXT='@EXEEXT@' srcdir='$(srcdir)' \ LOCALE_FR='@LOCALE_FR@' LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' \ LOCALE_FR='@LOCALE_FR@' LOCALE_TR_UTF8='@LOCALE_TR_UTF8@' \ LOCALE_FR='@LOCALE_FR@' LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' \ LOCALE_JA='@LOCALE_JA@' LOCALE_ZH_CN='@LOCALE_ZH_CN@' \ LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' LOCALE_FR='@LOCALE_FR@' \ LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' LOCALE_FR='@LOCALE_FR@' \ LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' LOCALE_JA='@LOCALE_JA@' \ LOCALE_ZH_CN='@LOCALE_ZH_CN@' MAKE='$(MAKE)' \ LOCALE_FR='@LOCALE_FR@' LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' \ LOCALE_JA='@LOCALE_JA@' LOCALE_ZH_CN='@LOCALE_ZH_CN@' noinst_HEADERS = noinst_LIBRARIES = check_LIBRARIES = libtests.a EXTRA_DIST = test-alloca-opt.c test-argp.c test-argp-2.sh \ test-binary-io.sh test-binary-io.c macros.h test-btowc1.sh \ test-btowc2.sh test-btowc.c signature.h macros.h \ test-c-ctype.c macros.h test-c-strcase.sh test-c-strcasecmp.c \ test-c-strncasecmp.c macros.h close.c test-close.c signature.h \ macros.h ctype.in.h test-ctype.c dup2.c test-dup2.c \ signature.h macros.h test-environ.c test-errno.c fcntl.in.h \ test-fcntl-h.c fd-hook.h fdopen.c test-fdopen.c signature.h \ macros.h test-fgetc.c signature.h macros.h flexmember.h \ test-float.c macros.h fpucw.h test-fputc.c signature.h \ macros.h test-fread.c signature.h macros.h fstat.c \ test-fstat.c signature.h macros.h test-fwrite.c signature.h \ macros.h getcwd-lgpl.c test-getcwd-lgpl.c signature.h macros.h \ getdtablesize.c test-getdtablesize.c signature.h macros.h \ macros.h signature.h test-getopt.c test-getopt.h \ test-getopt_long.h getpagesize.c test-getprogname.c \ gettimeofday.c signature.h test-gettimeofday.c ignore-value.h \ test-ignore-value.c test-intprops.c macros.h inttypes.in.h \ test-inttypes.c test-langinfo.c test-limits-h.c test-locale.c \ test-localeconv.c signature.h macros.h localename.h \ test-localename.c macros.h test-lock.c lstat.c test-lstat.h \ test-lstat.c signature.h macros.h test-malloc-gnu.c malloca.h \ malloca.valgrind test-malloca.c test-math.c macros.h \ test-mbrtowc1.sh test-mbrtowc2.sh test-mbrtowc3.sh \ test-mbrtowc4.sh test-mbrtowc5.sh test-mbrtowc.c \ test-mbrtowc-w32-1.sh test-mbrtowc-w32-2.sh \ test-mbrtowc-w32-3.sh test-mbrtowc-w32-4.sh \ test-mbrtowc-w32-5.sh test-mbrtowc-w32.c signature.h macros.h \ test-mbsinit.sh test-mbsinit.c signature.h macros.h \ test-memchr.c zerosize-ptr.h signature.h macros.h \ test-nl_langinfo.sh test-nl_langinfo.c signature.h macros.h \ open.c test-open.h test-open.c signature.h macros.h pathmax.h \ test-pathmax.c putenv.c test-rawmemchr.c zerosize-ptr.h \ signature.h macros.h test-regex.c macros.h same-inode.h \ setenv.c test-setenv.c signature.h macros.h setlocale.c \ test-setlocale1.sh test-setlocale1.c test-setlocale2.sh \ test-setlocale2.c signature.h macros.h test-sleep.c \ signature.h macros.h \ $(top_srcdir)/bootstrapped/build-aux/snippet/_Noreturn.h \ $(top_srcdir)/bootstrapped/build-aux/snippet/arg-nonnull.h \ $(top_srcdir)/bootstrapped/build-aux/snippet/c++defs.h \ $(top_srcdir)/bootstrapped/build-aux/snippet/warn-on-use.h \ stat.c test-stat.h test-stat.c signature.h macros.h \ test-stdalign.c macros.h test-stdbool.c test-stddef.c \ test-stdint.c test-stdio.c test-stdlib.c test-sys_wait.h \ test-strchrnul.c signature.h macros.h test-strerror.c \ signature.h macros.h test-string.c test-strings.c \ test-strnlen.c zerosize-ptr.h signature.h macros.h symlink.c \ test-symlink.h test-symlink.c signature.h macros.h \ sys_stat.in.h test-sys_stat.c sys_time.in.h test-sys_time.c \ test-sys_types.c test-sysexits.c init.sh test-init.sh \ test-thread_self.c test-thread_create.c macros.h time.in.h \ test-time.c test-unistd.c unsetenv.c test-unsetenv.c \ signature.h macros.h test-vasnprintf.c macros.h test-verify.c \ test-verify.sh test-vsnprintf.c signature.h macros.h \ test-wchar.c test-wcrtomb.sh test-wcrtomb.c \ test-wcrtomb-w32-1.sh test-wcrtomb-w32-2.sh \ test-wcrtomb-w32-3.sh test-wcrtomb-w32-4.sh \ test-wcrtomb-w32-5.sh test-wcrtomb-w32.c signature.h macros.h \ wctob.c wctomb-impl.h wctomb.c test-wctype-h.c macros.h # The BUILT_SOURCES created by this Makefile snippet are not used via #include # statements but through direct file reference. 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GENERATED AUTOMATICALLY! ## Process this file with automake to produce Makefile.in. # Copyright (C) 2002-2016 Free Software Foundation, Inc. # # This file is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This file is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this file. If not, see . # # As a special exception to the GNU General Public License, # this file may be distributed as part of a program that # contains a configuration script generated by Autoconf, under # the same distribution terms as the rest of that program. # # Generated by gnulib-tool. AUTOMAKE_OPTIONS = 1.9.6 foreign subdir-objects SUBDIRS = . TESTS = XFAIL_TESTS = TESTS_ENVIRONMENT = noinst_PROGRAMS = check_PROGRAMS = noinst_HEADERS = noinst_LIBRARIES = check_LIBRARIES = libtests.a EXTRA_DIST = BUILT_SOURCES = SUFFIXES = MOSTLYCLEANFILES = core *.stackdump MOSTLYCLEANDIRS = CLEANFILES = DISTCLEANFILES = MAINTAINERCLEANFILES = AM_CPPFLAGS = \ -D@gltests_WITNESS@=1 \ -I. -I$(srcdir) \ -I../.. -I$(srcdir)/../.. \ -I../../bootstrapped/lib -I$(srcdir)/../../bootstrapped/lib LDADD = libtests.a ../../bootstrapped/lib/libgnu.la libtests.a $(LIBTESTS_LIBDEPS) libtests_a_SOURCES = libtests_a_LIBADD = $(gltests_LIBOBJS) libtests_a_DEPENDENCIES = $(gltests_LIBOBJS) EXTRA_libtests_a_SOURCES = AM_LIBTOOLFLAGS = --preserve-dup-deps TESTS_ENVIRONMENT += EXEEXT='@EXEEXT@' srcdir='$(srcdir)' ## begin gnulib module alloca-opt-tests TESTS += test-alloca-opt check_PROGRAMS += test-alloca-opt EXTRA_DIST += test-alloca-opt.c ## end gnulib module alloca-opt-tests ## begin gnulib module argp-tests TESTS += test-argp test-argp-2.sh check_PROGRAMS += test-argp test_argp_LDADD = $(LDADD) @LIBINTL@ EXTRA_DIST += test-argp.c test-argp-2.sh ## end gnulib module argp-tests ## begin gnulib module binary-io libtests_a_SOURCES += binary-io.h binary-io.c ## end gnulib module binary-io ## begin gnulib module binary-io-tests TESTS += test-binary-io.sh check_PROGRAMS += test-binary-io EXTRA_DIST += test-binary-io.sh test-binary-io.c macros.h ## end gnulib module binary-io-tests ## begin gnulib module btowc-tests TESTS += test-btowc1.sh test-btowc2.sh TESTS_ENVIRONMENT += LOCALE_FR='@LOCALE_FR@' LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' check_PROGRAMS += test-btowc EXTRA_DIST += test-btowc1.sh test-btowc2.sh test-btowc.c signature.h macros.h ## end gnulib module btowc-tests ## begin gnulib module c-ctype-tests TESTS += test-c-ctype check_PROGRAMS += test-c-ctype EXTRA_DIST += test-c-ctype.c macros.h ## end gnulib module c-ctype-tests ## begin gnulib module c-strcase libtests_a_SOURCES += c-strcase.h c-strcasecmp.c c-strncasecmp.c ## end gnulib module c-strcase ## begin gnulib module c-strcase-tests TESTS += test-c-strcase.sh TESTS_ENVIRONMENT += LOCALE_FR='@LOCALE_FR@' LOCALE_TR_UTF8='@LOCALE_TR_UTF8@' check_PROGRAMS += test-c-strcasecmp test-c-strncasecmp EXTRA_DIST += test-c-strcase.sh test-c-strcasecmp.c test-c-strncasecmp.c macros.h ## end gnulib module c-strcase-tests ## begin gnulib module close EXTRA_DIST += close.c EXTRA_libtests_a_SOURCES += close.c ## end gnulib module close ## begin gnulib module close-tests TESTS += test-close check_PROGRAMS += test-close EXTRA_DIST += test-close.c signature.h macros.h ## end gnulib module close-tests ## begin gnulib module ctype BUILT_SOURCES += ctype.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. ctype.h: ctype.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_CTYPE_H''@|$(NEXT_CTYPE_H)|g' \ -e 's/@''GNULIB_ISBLANK''@/$(GNULIB_ISBLANK)/g' \ -e 's/@''HAVE_ISBLANK''@/$(HAVE_ISBLANK)/g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/ctype.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += ctype.h ctype.h-t EXTRA_DIST += ctype.in.h ## end gnulib module ctype ## begin gnulib module ctype-tests TESTS += test-ctype check_PROGRAMS += test-ctype EXTRA_DIST += test-ctype.c ## end gnulib module ctype-tests ## begin gnulib module dup2 EXTRA_DIST += dup2.c EXTRA_libtests_a_SOURCES += dup2.c ## end gnulib module dup2 ## begin gnulib module dup2-tests TESTS += test-dup2 check_PROGRAMS += test-dup2 EXTRA_DIST += test-dup2.c signature.h macros.h ## end gnulib module dup2-tests ## begin gnulib module environ-tests TESTS += test-environ check_PROGRAMS += test-environ EXTRA_DIST += test-environ.c ## end gnulib module environ-tests ## begin gnulib module errno-tests TESTS += test-errno check_PROGRAMS += test-errno EXTRA_DIST += test-errno.c ## end gnulib module errno-tests ## begin gnulib module fcntl-h BUILT_SOURCES += fcntl.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. fcntl.h: fcntl.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_FCNTL_H''@|$(NEXT_FCNTL_H)|g' \ -e 's/@''GNULIB_FCNTL''@/$(GNULIB_FCNTL)/g' \ -e 's/@''GNULIB_NONBLOCKING''@/$(GNULIB_NONBLOCKING)/g' \ -e 's/@''GNULIB_OPEN''@/$(GNULIB_OPEN)/g' \ -e 's/@''GNULIB_OPENAT''@/$(GNULIB_OPENAT)/g' \ -e 's|@''HAVE_FCNTL''@|$(HAVE_FCNTL)|g' \ -e 's|@''HAVE_OPENAT''@|$(HAVE_OPENAT)|g' \ -e 's|@''REPLACE_FCNTL''@|$(REPLACE_FCNTL)|g' \ -e 's|@''REPLACE_OPEN''@|$(REPLACE_OPEN)|g' \ -e 's|@''REPLACE_OPENAT''@|$(REPLACE_OPENAT)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/fcntl.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += fcntl.h fcntl.h-t EXTRA_DIST += fcntl.in.h ## end gnulib module fcntl-h ## begin gnulib module fcntl-h-tests TESTS += test-fcntl-h check_PROGRAMS += test-fcntl-h EXTRA_DIST += test-fcntl-h.c ## end gnulib module fcntl-h-tests ## begin gnulib module fd-hook libtests_a_SOURCES += fd-hook.c EXTRA_DIST += fd-hook.h ## end gnulib module fd-hook ## begin gnulib module fdopen EXTRA_DIST += fdopen.c EXTRA_libtests_a_SOURCES += fdopen.c ## end gnulib module fdopen ## begin gnulib module fdopen-tests TESTS += test-fdopen check_PROGRAMS += test-fdopen EXTRA_DIST += test-fdopen.c signature.h macros.h ## end gnulib module fdopen-tests ## begin gnulib module fgetc-tests TESTS += test-fgetc check_PROGRAMS += test-fgetc EXTRA_DIST += test-fgetc.c signature.h macros.h ## end gnulib module fgetc-tests ## begin gnulib module flexmember EXTRA_DIST += flexmember.h ## end gnulib module flexmember ## begin gnulib module float-tests TESTS += test-float check_PROGRAMS += test-float EXTRA_DIST += test-float.c macros.h ## end gnulib module float-tests ## begin gnulib module fpucw EXTRA_DIST += fpucw.h ## end gnulib module fpucw ## begin gnulib module fputc-tests TESTS += test-fputc check_PROGRAMS += test-fputc EXTRA_DIST += test-fputc.c signature.h macros.h ## end gnulib module fputc-tests ## begin gnulib module fread-tests TESTS += test-fread check_PROGRAMS += test-fread EXTRA_DIST += test-fread.c signature.h macros.h ## end gnulib module fread-tests ## begin gnulib module fstat EXTRA_DIST += fstat.c EXTRA_libtests_a_SOURCES += fstat.c ## end gnulib module fstat ## begin gnulib module fstat-tests TESTS += test-fstat check_PROGRAMS += test-fstat EXTRA_DIST += test-fstat.c signature.h macros.h ## end gnulib module fstat-tests ## begin gnulib module fwrite-tests TESTS += test-fwrite check_PROGRAMS += test-fwrite EXTRA_DIST += test-fwrite.c signature.h macros.h ## end gnulib module fwrite-tests ## begin gnulib module getcwd-lgpl EXTRA_DIST += getcwd-lgpl.c EXTRA_libtests_a_SOURCES += getcwd-lgpl.c ## end gnulib module getcwd-lgpl ## begin gnulib module getcwd-lgpl-tests TESTS += test-getcwd-lgpl check_PROGRAMS += test-getcwd-lgpl test_getcwd_lgpl_LDADD = $(LDADD) $(LIBINTL) EXTRA_DIST += test-getcwd-lgpl.c signature.h macros.h ## end gnulib module getcwd-lgpl-tests ## begin gnulib module getdtablesize EXTRA_DIST += getdtablesize.c EXTRA_libtests_a_SOURCES += getdtablesize.c ## end gnulib module getdtablesize ## begin gnulib module getdtablesize-tests TESTS += test-getdtablesize check_PROGRAMS += test-getdtablesize EXTRA_DIST += test-getdtablesize.c signature.h macros.h ## end gnulib module getdtablesize-tests ## begin gnulib module getopt-posix-tests TESTS += test-getopt check_PROGRAMS += test-getopt test_getopt_LDADD = $(LDADD) $(LIBINTL) EXTRA_DIST += macros.h signature.h test-getopt.c test-getopt.h test-getopt_long.h ## end gnulib module getopt-posix-tests ## begin gnulib module getpagesize EXTRA_DIST += getpagesize.c EXTRA_libtests_a_SOURCES += getpagesize.c ## end gnulib module getpagesize ## begin gnulib module getprogname-tests DEFS += -DEXEEXT=\"@EXEEXT@\" TESTS += test-getprogname check_PROGRAMS += test-getprogname test_getprogname_LDADD = $(LDADD) EXTRA_DIST += test-getprogname.c ## end gnulib module getprogname-tests ## begin gnulib module gettimeofday EXTRA_DIST += gettimeofday.c EXTRA_libtests_a_SOURCES += gettimeofday.c ## end gnulib module gettimeofday ## begin gnulib module gettimeofday-tests TESTS += test-gettimeofday check_PROGRAMS += test-gettimeofday EXTRA_DIST += signature.h test-gettimeofday.c ## end gnulib module gettimeofday-tests ## begin gnulib module ignore-value EXTRA_DIST += ignore-value.h ## end gnulib module ignore-value ## begin gnulib module ignore-value-tests TESTS += test-ignore-value check_PROGRAMS += test-ignore-value EXTRA_DIST += test-ignore-value.c ## end gnulib module ignore-value-tests ## begin gnulib module intprops-tests TESTS += test-intprops check_PROGRAMS += test-intprops EXTRA_DIST += test-intprops.c macros.h ## end gnulib module intprops-tests ## begin gnulib module inttypes-incomplete BUILT_SOURCES += inttypes.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. inttypes.h: inttypes.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(ARG_NONNULL_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's/@''HAVE_INTTYPES_H''@/$(HAVE_INTTYPES_H)/g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_INTTYPES_H''@|$(NEXT_INTTYPES_H)|g' \ -e 's/@''PRI_MACROS_BROKEN''@/$(PRI_MACROS_BROKEN)/g' \ -e 's/@''APPLE_UNIVERSAL_BUILD''@/$(APPLE_UNIVERSAL_BUILD)/g' \ -e 's/@''HAVE_LONG_LONG_INT''@/$(HAVE_LONG_LONG_INT)/g' \ -e 's/@''HAVE_UNSIGNED_LONG_LONG_INT''@/$(HAVE_UNSIGNED_LONG_LONG_INT)/g' \ -e 's/@''PRIPTR_PREFIX''@/$(PRIPTR_PREFIX)/g' \ -e 's/@''GNULIB_IMAXABS''@/$(GNULIB_IMAXABS)/g' \ -e 's/@''GNULIB_IMAXDIV''@/$(GNULIB_IMAXDIV)/g' \ -e 's/@''GNULIB_STRTOIMAX''@/$(GNULIB_STRTOIMAX)/g' \ -e 's/@''GNULIB_STRTOUMAX''@/$(GNULIB_STRTOUMAX)/g' \ -e 's/@''HAVE_DECL_IMAXABS''@/$(HAVE_DECL_IMAXABS)/g' \ -e 's/@''HAVE_DECL_IMAXDIV''@/$(HAVE_DECL_IMAXDIV)/g' \ -e 's/@''HAVE_DECL_STRTOIMAX''@/$(HAVE_DECL_STRTOIMAX)/g' \ -e 's/@''HAVE_DECL_STRTOUMAX''@/$(HAVE_DECL_STRTOUMAX)/g' \ -e 's/@''REPLACE_STRTOIMAX''@/$(REPLACE_STRTOIMAX)/g' \ -e 's/@''REPLACE_STRTOUMAX''@/$(REPLACE_STRTOUMAX)/g' \ -e 's/@''INT32_MAX_LT_INTMAX_MAX''@/$(INT32_MAX_LT_INTMAX_MAX)/g' \ -e 's/@''INT64_MAX_EQ_LONG_MAX''@/$(INT64_MAX_EQ_LONG_MAX)/g' \ -e 's/@''UINT32_MAX_LT_UINTMAX_MAX''@/$(UINT32_MAX_LT_UINTMAX_MAX)/g' \ -e 's/@''UINT64_MAX_EQ_ULONG_MAX''@/$(UINT64_MAX_EQ_ULONG_MAX)/g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/inttypes.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += inttypes.h inttypes.h-t EXTRA_DIST += inttypes.in.h ## end gnulib module inttypes-incomplete ## begin gnulib module inttypes-tests TESTS += test-inttypes check_PROGRAMS += test-inttypes EXTRA_DIST += test-inttypes.c ## end gnulib module inttypes-tests ## begin gnulib module langinfo-tests TESTS += test-langinfo check_PROGRAMS += test-langinfo EXTRA_DIST += test-langinfo.c ## end gnulib module langinfo-tests ## begin gnulib module limits-h-tests TESTS += test-limits-h check_PROGRAMS += test-limits-h EXTRA_DIST += test-limits-h.c ## end gnulib module limits-h-tests ## begin gnulib module locale-tests TESTS += test-locale check_PROGRAMS += test-locale EXTRA_DIST += test-locale.c ## end gnulib module locale-tests ## begin gnulib module localeconv-tests TESTS += test-localeconv check_PROGRAMS += test-localeconv EXTRA_DIST += test-localeconv.c signature.h macros.h ## end gnulib module localeconv-tests ## begin gnulib module localename libtests_a_SOURCES += localename.c EXTRA_DIST += localename.h ## end gnulib module localename ## begin gnulib module localename-tests TESTS += test-localename check_PROGRAMS += test-localename test_localename_LDADD = $(LDADD) @INTL_MACOSX_LIBS@ $(LIBTHREAD) EXTRA_DIST += test-localename.c macros.h ## end gnulib module localename-tests ## begin gnulib module lock-tests TESTS += test-lock check_PROGRAMS += test-lock test_lock_LDADD = $(LDADD) @LIBMULTITHREAD@ @YIELD_LIB@ EXTRA_DIST += test-lock.c ## end gnulib module lock-tests ## begin gnulib module lstat EXTRA_DIST += lstat.c EXTRA_libtests_a_SOURCES += lstat.c ## end gnulib module lstat ## begin gnulib module lstat-tests TESTS += test-lstat check_PROGRAMS += test-lstat EXTRA_DIST += test-lstat.h test-lstat.c signature.h macros.h ## end gnulib module lstat-tests ## begin gnulib module malloc-gnu-tests TESTS += test-malloc-gnu check_PROGRAMS += test-malloc-gnu EXTRA_DIST += test-malloc-gnu.c ## end gnulib module malloc-gnu-tests ## begin gnulib module malloca libtests_a_SOURCES += malloca.c EXTRA_DIST += malloca.h malloca.valgrind ## end gnulib module malloca ## begin gnulib module malloca-tests TESTS += test-malloca check_PROGRAMS += test-malloca EXTRA_DIST += test-malloca.c ## end gnulib module malloca-tests ## begin gnulib module math-tests TESTS += test-math check_PROGRAMS += test-math EXTRA_DIST += test-math.c macros.h ## end gnulib module math-tests ## begin gnulib module mbrtowc-tests TESTS += \ test-mbrtowc1.sh test-mbrtowc2.sh test-mbrtowc3.sh test-mbrtowc4.sh \ test-mbrtowc5.sh \ test-mbrtowc-w32-1.sh test-mbrtowc-w32-2.sh test-mbrtowc-w32-3.sh \ test-mbrtowc-w32-4.sh test-mbrtowc-w32-5.sh TESTS_ENVIRONMENT += \ LOCALE_FR='@LOCALE_FR@' \ LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' \ LOCALE_JA='@LOCALE_JA@' \ LOCALE_ZH_CN='@LOCALE_ZH_CN@' check_PROGRAMS += test-mbrtowc test-mbrtowc-w32 EXTRA_DIST += test-mbrtowc1.sh test-mbrtowc2.sh test-mbrtowc3.sh test-mbrtowc4.sh test-mbrtowc5.sh test-mbrtowc.c test-mbrtowc-w32-1.sh test-mbrtowc-w32-2.sh test-mbrtowc-w32-3.sh test-mbrtowc-w32-4.sh test-mbrtowc-w32-5.sh test-mbrtowc-w32.c signature.h macros.h ## end gnulib module mbrtowc-tests ## begin gnulib module mbsinit-tests TESTS += test-mbsinit.sh TESTS_ENVIRONMENT += LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' check_PROGRAMS += test-mbsinit EXTRA_DIST += test-mbsinit.sh test-mbsinit.c signature.h macros.h ## end gnulib module mbsinit-tests ## begin gnulib module memchr-tests TESTS += test-memchr check_PROGRAMS += test-memchr EXTRA_DIST += test-memchr.c zerosize-ptr.h signature.h macros.h ## end gnulib module memchr-tests ## begin gnulib module nl_langinfo-tests TESTS += test-nl_langinfo.sh TESTS_ENVIRONMENT += LOCALE_FR='@LOCALE_FR@' LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' check_PROGRAMS += test-nl_langinfo EXTRA_DIST += test-nl_langinfo.sh test-nl_langinfo.c signature.h macros.h ## end gnulib module nl_langinfo-tests ## begin gnulib module open EXTRA_DIST += open.c EXTRA_libtests_a_SOURCES += open.c ## end gnulib module open ## begin gnulib module open-tests TESTS += test-open check_PROGRAMS += test-open EXTRA_DIST += test-open.h test-open.c signature.h macros.h ## end gnulib module open-tests ## begin gnulib module pathmax EXTRA_DIST += pathmax.h ## end gnulib module pathmax ## begin gnulib module pathmax-tests TESTS += test-pathmax check_PROGRAMS += test-pathmax EXTRA_DIST += test-pathmax.c ## end gnulib module pathmax-tests ## begin gnulib module putenv EXTRA_DIST += putenv.c EXTRA_libtests_a_SOURCES += putenv.c ## end gnulib module putenv ## begin gnulib module rawmemchr-tests TESTS += test-rawmemchr check_PROGRAMS += test-rawmemchr EXTRA_DIST += test-rawmemchr.c zerosize-ptr.h signature.h macros.h ## end gnulib module rawmemchr-tests ## begin gnulib module regex-tests TESTS += test-regex check_PROGRAMS += test-regex test_regex_LDADD = $(LDADD) @LIBINTL@ $(LIBTHREAD) $(LIB_PTHREAD) EXTRA_DIST += test-regex.c macros.h ## end gnulib module regex-tests ## begin gnulib module same-inode EXTRA_DIST += same-inode.h ## end gnulib module same-inode ## begin gnulib module setenv EXTRA_DIST += setenv.c EXTRA_libtests_a_SOURCES += setenv.c ## end gnulib module setenv ## begin gnulib module setenv-tests TESTS += test-setenv check_PROGRAMS += test-setenv EXTRA_DIST += test-setenv.c signature.h macros.h ## end gnulib module setenv-tests ## begin gnulib module setlocale EXTRA_DIST += setlocale.c EXTRA_libtests_a_SOURCES += setlocale.c ## end gnulib module setlocale ## begin gnulib module setlocale-tests TESTS += test-setlocale1.sh test-setlocale2.sh TESTS_ENVIRONMENT += \ LOCALE_FR='@LOCALE_FR@' \ LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' \ LOCALE_JA='@LOCALE_JA@' \ LOCALE_ZH_CN='@LOCALE_ZH_CN@' check_PROGRAMS += test-setlocale1 test-setlocale2 EXTRA_DIST += test-setlocale1.sh test-setlocale1.c test-setlocale2.sh test-setlocale2.c signature.h macros.h ## end gnulib module setlocale-tests ## begin gnulib module sleep-tests TESTS += test-sleep check_PROGRAMS += test-sleep EXTRA_DIST += test-sleep.c signature.h macros.h ## end gnulib module sleep-tests ## begin gnulib module snippet/_Noreturn # Because this Makefile snippet defines a variable used by other # gnulib Makefile snippets, it must be present in all Makefile.am that # need it. This is ensured by the applicability 'all' defined above. _NORETURN_H=$(top_srcdir)/bootstrapped/build-aux/snippet/_Noreturn.h EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/snippet/_Noreturn.h ## end gnulib module snippet/_Noreturn ## begin gnulib module snippet/arg-nonnull # The BUILT_SOURCES created by this Makefile snippet are not used via #include # statements but through direct file reference. Therefore this snippet must be # present in all Makefile.am that need it. This is ensured by the applicability # 'all' defined above. BUILT_SOURCES += arg-nonnull.h # The arg-nonnull.h that gets inserted into generated .h files is the same as # build-aux/snippet/arg-nonnull.h, except that it has the copyright header cut # off. arg-nonnull.h: $(top_srcdir)/bootstrapped/build-aux/snippet/arg-nonnull.h $(AM_V_GEN)rm -f $@-t $@ && \ sed -n -e '/GL_ARG_NONNULL/,$$p' \ < $(top_srcdir)/bootstrapped/build-aux/snippet/arg-nonnull.h \ > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += arg-nonnull.h arg-nonnull.h-t ARG_NONNULL_H=arg-nonnull.h EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/snippet/arg-nonnull.h ## end gnulib module snippet/arg-nonnull ## begin gnulib module snippet/c++defs # The BUILT_SOURCES created by this Makefile snippet are not used via #include # statements but through direct file reference. Therefore this snippet must be # present in all Makefile.am that need it. This is ensured by the applicability # 'all' defined above. BUILT_SOURCES += c++defs.h # The c++defs.h that gets inserted into generated .h files is the same as # build-aux/snippet/c++defs.h, except that it has the copyright header cut off. c++defs.h: $(top_srcdir)/bootstrapped/build-aux/snippet/c++defs.h $(AM_V_GEN)rm -f $@-t $@ && \ sed -n -e '/_GL_CXXDEFS/,$$p' \ < $(top_srcdir)/bootstrapped/build-aux/snippet/c++defs.h \ > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += c++defs.h c++defs.h-t CXXDEFS_H=c++defs.h EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/snippet/c++defs.h ## end gnulib module snippet/c++defs ## begin gnulib module snippet/warn-on-use BUILT_SOURCES += warn-on-use.h # The warn-on-use.h that gets inserted into generated .h files is the same as # build-aux/snippet/warn-on-use.h, except that it has the copyright header cut # off. warn-on-use.h: $(top_srcdir)/bootstrapped/build-aux/snippet/warn-on-use.h $(AM_V_GEN)rm -f $@-t $@ && \ sed -n -e '/^.ifndef/,$$p' \ < $(top_srcdir)/bootstrapped/build-aux/snippet/warn-on-use.h \ > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += warn-on-use.h warn-on-use.h-t WARN_ON_USE_H=warn-on-use.h EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/snippet/warn-on-use.h ## end gnulib module snippet/warn-on-use ## begin gnulib module stat EXTRA_DIST += stat.c EXTRA_libtests_a_SOURCES += stat.c ## end gnulib module stat ## begin gnulib module stat-tests TESTS += test-stat check_PROGRAMS += test-stat test_stat_LDADD = $(LDADD) $(LIBINTL) EXTRA_DIST += test-stat.h test-stat.c signature.h macros.h ## end gnulib module stat-tests ## begin gnulib module stdalign-tests TESTS += test-stdalign check_PROGRAMS += test-stdalign EXTRA_DIST += test-stdalign.c macros.h ## end gnulib module stdalign-tests ## begin gnulib module stdbool-tests TESTS += test-stdbool check_PROGRAMS += test-stdbool EXTRA_DIST += test-stdbool.c ## end gnulib module stdbool-tests ## begin gnulib module stddef-tests TESTS += test-stddef check_PROGRAMS += test-stddef EXTRA_DIST += test-stddef.c ## end gnulib module stddef-tests ## begin gnulib module stdint-tests TESTS += test-stdint check_PROGRAMS += test-stdint EXTRA_DIST += test-stdint.c ## end gnulib module stdint-tests ## begin gnulib module stdio-tests TESTS += test-stdio check_PROGRAMS += test-stdio EXTRA_DIST += test-stdio.c ## end gnulib module stdio-tests ## begin gnulib module stdlib-tests TESTS += test-stdlib check_PROGRAMS += test-stdlib EXTRA_DIST += test-stdlib.c test-sys_wait.h ## end gnulib module stdlib-tests ## begin gnulib module strchrnul-tests TESTS += test-strchrnul check_PROGRAMS += test-strchrnul EXTRA_DIST += test-strchrnul.c signature.h macros.h ## end gnulib module strchrnul-tests ## begin gnulib module strerror-tests TESTS += test-strerror check_PROGRAMS += test-strerror EXTRA_DIST += test-strerror.c signature.h macros.h ## end gnulib module strerror-tests ## begin gnulib module string-tests TESTS += test-string check_PROGRAMS += test-string EXTRA_DIST += test-string.c ## end gnulib module string-tests ## begin gnulib module strings-tests TESTS += test-strings check_PROGRAMS += test-strings EXTRA_DIST += test-strings.c ## end gnulib module strings-tests ## begin gnulib module strnlen-tests TESTS += test-strnlen check_PROGRAMS += test-strnlen EXTRA_DIST += test-strnlen.c zerosize-ptr.h signature.h macros.h ## end gnulib module strnlen-tests ## begin gnulib module symlink EXTRA_DIST += symlink.c EXTRA_libtests_a_SOURCES += symlink.c ## end gnulib module symlink ## begin gnulib module symlink-tests TESTS += test-symlink check_PROGRAMS += test-symlink EXTRA_DIST += test-symlink.h test-symlink.c signature.h macros.h ## end gnulib module symlink-tests ## begin gnulib module sys_stat BUILT_SOURCES += sys/stat.h # We need the following in order to create when the system # has one that is incomplete. sys/stat.h: sys_stat.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_at)$(MKDIR_P) sys $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_SYS_STAT_H''@|$(NEXT_SYS_STAT_H)|g' \ -e 's|@''WINDOWS_64_BIT_ST_SIZE''@|$(WINDOWS_64_BIT_ST_SIZE)|g' \ -e 's/@''GNULIB_FCHMODAT''@/$(GNULIB_FCHMODAT)/g' \ -e 's/@''GNULIB_FSTAT''@/$(GNULIB_FSTAT)/g' \ -e 's/@''GNULIB_FSTATAT''@/$(GNULIB_FSTATAT)/g' \ -e 's/@''GNULIB_FUTIMENS''@/$(GNULIB_FUTIMENS)/g' \ -e 's/@''GNULIB_LCHMOD''@/$(GNULIB_LCHMOD)/g' \ -e 's/@''GNULIB_LSTAT''@/$(GNULIB_LSTAT)/g' \ -e 's/@''GNULIB_MKDIRAT''@/$(GNULIB_MKDIRAT)/g' \ -e 's/@''GNULIB_MKFIFO''@/$(GNULIB_MKFIFO)/g' \ -e 's/@''GNULIB_MKFIFOAT''@/$(GNULIB_MKFIFOAT)/g' \ -e 's/@''GNULIB_MKNOD''@/$(GNULIB_MKNOD)/g' \ -e 's/@''GNULIB_MKNODAT''@/$(GNULIB_MKNODAT)/g' \ -e 's/@''GNULIB_STAT''@/$(GNULIB_STAT)/g' \ -e 's/@''GNULIB_UTIMENSAT''@/$(GNULIB_UTIMENSAT)/g' \ -e 's|@''HAVE_FCHMODAT''@|$(HAVE_FCHMODAT)|g' \ -e 's|@''HAVE_FSTATAT''@|$(HAVE_FSTATAT)|g' \ -e 's|@''HAVE_FUTIMENS''@|$(HAVE_FUTIMENS)|g' \ -e 's|@''HAVE_LCHMOD''@|$(HAVE_LCHMOD)|g' \ -e 's|@''HAVE_LSTAT''@|$(HAVE_LSTAT)|g' \ -e 's|@''HAVE_MKDIRAT''@|$(HAVE_MKDIRAT)|g' \ -e 's|@''HAVE_MKFIFO''@|$(HAVE_MKFIFO)|g' \ -e 's|@''HAVE_MKFIFOAT''@|$(HAVE_MKFIFOAT)|g' \ -e 's|@''HAVE_MKNOD''@|$(HAVE_MKNOD)|g' \ -e 's|@''HAVE_MKNODAT''@|$(HAVE_MKNODAT)|g' \ -e 's|@''HAVE_UTIMENSAT''@|$(HAVE_UTIMENSAT)|g' \ -e 's|@''REPLACE_FSTAT''@|$(REPLACE_FSTAT)|g' \ -e 's|@''REPLACE_FSTATAT''@|$(REPLACE_FSTATAT)|g' \ -e 's|@''REPLACE_FUTIMENS''@|$(REPLACE_FUTIMENS)|g' \ -e 's|@''REPLACE_LSTAT''@|$(REPLACE_LSTAT)|g' \ -e 's|@''REPLACE_MKDIR''@|$(REPLACE_MKDIR)|g' \ -e 's|@''REPLACE_MKFIFO''@|$(REPLACE_MKFIFO)|g' \ -e 's|@''REPLACE_MKNOD''@|$(REPLACE_MKNOD)|g' \ -e 's|@''REPLACE_STAT''@|$(REPLACE_STAT)|g' \ -e 's|@''REPLACE_UTIMENSAT''@|$(REPLACE_UTIMENSAT)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/sys_stat.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += sys/stat.h sys/stat.h-t MOSTLYCLEANDIRS += sys EXTRA_DIST += sys_stat.in.h ## end gnulib module sys_stat ## begin gnulib module sys_stat-tests TESTS += test-sys_stat check_PROGRAMS += test-sys_stat EXTRA_DIST += test-sys_stat.c ## end gnulib module sys_stat-tests ## begin gnulib module sys_time BUILT_SOURCES += sys/time.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. sys/time.h: sys_time.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_at)$(MKDIR_P) sys $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's/@''HAVE_SYS_TIME_H''@/$(HAVE_SYS_TIME_H)/g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_SYS_TIME_H''@|$(NEXT_SYS_TIME_H)|g' \ -e 's/@''GNULIB_GETTIMEOFDAY''@/$(GNULIB_GETTIMEOFDAY)/g' \ -e 's|@''HAVE_WINSOCK2_H''@|$(HAVE_WINSOCK2_H)|g' \ -e 's/@''HAVE_GETTIMEOFDAY''@/$(HAVE_GETTIMEOFDAY)/g' \ -e 's/@''HAVE_STRUCT_TIMEVAL''@/$(HAVE_STRUCT_TIMEVAL)/g' \ -e 's/@''REPLACE_GETTIMEOFDAY''@/$(REPLACE_GETTIMEOFDAY)/g' \ -e 's/@''REPLACE_STRUCT_TIMEVAL''@/$(REPLACE_STRUCT_TIMEVAL)/g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/sys_time.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += sys/time.h sys/time.h-t EXTRA_DIST += sys_time.in.h ## end gnulib module sys_time ## begin gnulib module sys_time-tests TESTS += test-sys_time check_PROGRAMS += test-sys_time EXTRA_DIST += test-sys_time.c ## end gnulib module sys_time-tests ## begin gnulib module sys_types-tests TESTS += test-sys_types check_PROGRAMS += test-sys_types EXTRA_DIST += test-sys_types.c ## end gnulib module sys_types-tests ## begin gnulib module sysexits-tests TESTS += test-sysexits check_PROGRAMS += test-sysexits EXTRA_DIST += test-sysexits.c ## end gnulib module sysexits-tests ## begin gnulib module test-framework-sh-tests TESTS += test-init.sh EXTRA_DIST += init.sh EXTRA_DIST += test-init.sh ## end gnulib module test-framework-sh-tests ## begin gnulib module thread libtests_a_SOURCES += glthread/thread.h glthread/thread.c ## end gnulib module thread ## begin gnulib module thread-tests TESTS += test-thread_self test-thread_create check_PROGRAMS += test-thread_self test-thread_create test_thread_self_LDADD = $(LDADD) @LIBTHREAD@ test_thread_create_LDADD = $(LDADD) @LIBMULTITHREAD@ EXTRA_DIST += test-thread_self.c test-thread_create.c macros.h ## end gnulib module thread-tests ## begin gnulib module time BUILT_SOURCES += time.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. time.h: time.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_TIME_H''@|$(NEXT_TIME_H)|g' \ -e 's/@''GNULIB_GETTIMEOFDAY''@/$(GNULIB_GETTIMEOFDAY)/g' \ -e 's/@''GNULIB_MKTIME''@/$(GNULIB_MKTIME)/g' \ -e 's/@''GNULIB_NANOSLEEP''@/$(GNULIB_NANOSLEEP)/g' \ -e 's/@''GNULIB_STRPTIME''@/$(GNULIB_STRPTIME)/g' \ -e 's/@''GNULIB_TIMEGM''@/$(GNULIB_TIMEGM)/g' \ -e 's/@''GNULIB_TIME_R''@/$(GNULIB_TIME_R)/g' \ -e 's/@''GNULIB_TIME_RZ''@/$(GNULIB_TIME_RZ)/g' \ -e 's|@''HAVE_DECL_LOCALTIME_R''@|$(HAVE_DECL_LOCALTIME_R)|g' \ -e 's|@''HAVE_NANOSLEEP''@|$(HAVE_NANOSLEEP)|g' \ -e 's|@''HAVE_STRPTIME''@|$(HAVE_STRPTIME)|g' \ -e 's|@''HAVE_TIMEGM''@|$(HAVE_TIMEGM)|g' \ -e 's|@''HAVE_TIMEZONE_T''@|$(HAVE_TIMEZONE_T)|g' \ -e 's|@''REPLACE_GMTIME''@|$(REPLACE_GMTIME)|g' \ -e 's|@''REPLACE_LOCALTIME''@|$(REPLACE_LOCALTIME)|g' \ -e 's|@''REPLACE_LOCALTIME_R''@|$(REPLACE_LOCALTIME_R)|g' \ -e 's|@''REPLACE_MKTIME''@|$(REPLACE_MKTIME)|g' \ -e 's|@''REPLACE_NANOSLEEP''@|$(REPLACE_NANOSLEEP)|g' \ -e 's|@''REPLACE_TIMEGM''@|$(REPLACE_TIMEGM)|g' \ -e 's|@''PTHREAD_H_DEFINES_STRUCT_TIMESPEC''@|$(PTHREAD_H_DEFINES_STRUCT_TIMESPEC)|g' \ -e 's|@''SYS_TIME_H_DEFINES_STRUCT_TIMESPEC''@|$(SYS_TIME_H_DEFINES_STRUCT_TIMESPEC)|g' \ -e 's|@''TIME_H_DEFINES_STRUCT_TIMESPEC''@|$(TIME_H_DEFINES_STRUCT_TIMESPEC)|g' \ -e 's|@''UNISTD_H_DEFINES_STRUCT_TIMESPEC''@|$(UNISTD_H_DEFINES_STRUCT_TIMESPEC)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/time.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += time.h time.h-t EXTRA_DIST += time.in.h ## end gnulib module time ## begin gnulib module time-tests TESTS += test-time check_PROGRAMS += test-time EXTRA_DIST += test-time.c ## end gnulib module time-tests ## begin gnulib module unistd-tests TESTS += test-unistd check_PROGRAMS += test-unistd EXTRA_DIST += test-unistd.c ## end gnulib module unistd-tests ## begin gnulib module unsetenv EXTRA_DIST += unsetenv.c EXTRA_libtests_a_SOURCES += unsetenv.c ## end gnulib module unsetenv ## begin gnulib module unsetenv-tests TESTS += test-unsetenv check_PROGRAMS += test-unsetenv EXTRA_DIST += test-unsetenv.c signature.h macros.h ## end gnulib module unsetenv-tests ## begin gnulib module vasnprintf-tests TESTS += test-vasnprintf check_PROGRAMS += test-vasnprintf EXTRA_DIST += test-vasnprintf.c macros.h ## end gnulib module vasnprintf-tests ## begin gnulib module verify-tests TESTS_ENVIRONMENT += MAKE='$(MAKE)' TESTS += test-verify test-verify.sh check_PROGRAMS += test-verify # This test expects compilation of test-verify.c to fail, and # each time it fails, the makefile rule does not perform the usual # "mv -f $name.Tpo $name.po, so tell make clean to remove that file. MOSTLYCLEANFILES += .deps/test-verify.Tpo EXTRA_DIST += test-verify.c test-verify.sh ## end gnulib module verify-tests ## begin gnulib module vsnprintf-tests TESTS += test-vsnprintf check_PROGRAMS += test-vsnprintf EXTRA_DIST += test-vsnprintf.c signature.h macros.h ## end gnulib module vsnprintf-tests ## begin gnulib module wchar-tests TESTS += test-wchar check_PROGRAMS += test-wchar EXTRA_DIST += test-wchar.c ## end gnulib module wchar-tests ## begin gnulib module wcrtomb-tests TESTS += \ test-wcrtomb.sh \ test-wcrtomb-w32-1.sh test-wcrtomb-w32-2.sh test-wcrtomb-w32-3.sh \ test-wcrtomb-w32-4.sh test-wcrtomb-w32-5.sh TESTS_ENVIRONMENT += \ LOCALE_FR='@LOCALE_FR@' \ LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' \ LOCALE_JA='@LOCALE_JA@' \ LOCALE_ZH_CN='@LOCALE_ZH_CN@' check_PROGRAMS += test-wcrtomb test-wcrtomb-w32 EXTRA_DIST += test-wcrtomb.sh test-wcrtomb.c test-wcrtomb-w32-1.sh test-wcrtomb-w32-2.sh test-wcrtomb-w32-3.sh test-wcrtomb-w32-4.sh test-wcrtomb-w32-5.sh test-wcrtomb-w32.c signature.h macros.h ## end gnulib module wcrtomb-tests ## begin gnulib module wctob EXTRA_DIST += wctob.c EXTRA_libtests_a_SOURCES += wctob.c ## end gnulib module wctob ## begin gnulib module wctomb EXTRA_DIST += wctomb-impl.h wctomb.c EXTRA_libtests_a_SOURCES += wctomb.c ## end gnulib module wctomb ## begin gnulib module wctype-h-tests TESTS += test-wctype-h check_PROGRAMS += test-wctype-h EXTRA_DIST += test-wctype-h.c macros.h ## end gnulib module wctype-h-tests ## begin gnulib module yield libtests_a_SOURCES += glthread/yield.h ## end gnulib module yield # Clean up after Solaris cc. clean-local: rm -rf SunWS_cache mostlyclean-local: mostlyclean-generic @for dir in '' $(MOSTLYCLEANDIRS); do \ if test -n "$$dir" && test -d $$dir; then \ echo "rmdir $$dir"; rmdir $$dir; \ fi; \ done; \ : gnuastro-0.2.33-8a3b/bootstrapped/tests/glthread/0000755000175000017500000000000013004464723016642 500000000000000gnuastro-0.2.33-8a3b/bootstrapped/tests/glthread/yield.h0000644000175000017500000000474713004436755020061 00000000000000/* Yielding the processor to other threads and processes. Copyright (C) 2005-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* This file contains a primitive for yielding the processor to other threads. extern void gl_thread_yield (void); */ #ifndef _GLTHREAD_YIELD_H #define _GLTHREAD_YIELD_H #include /* ========================================================================= */ #if USE_POSIX_THREADS /* Use the POSIX threads library. */ # include # ifdef __cplusplus extern "C" { # endif # define gl_thread_yield() \ sched_yield () # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_PTH_THREADS /* Use the GNU Pth threads library. */ # include # ifdef __cplusplus extern "C" { # endif # define gl_thread_yield() \ pth_yield (NULL) # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_SOLARIS_THREADS /* Use the old Solaris threads library. */ # include # ifdef __cplusplus extern "C" { # endif # define gl_thread_yield() \ thr_yield () # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_WINDOWS_THREADS # define WIN32_LEAN_AND_MEAN /* avoid including junk */ # include # ifdef __cplusplus extern "C" { # endif # define gl_thread_yield() \ Sleep (0) # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if !(USE_POSIX_THREADS || USE_PTH_THREADS || USE_SOLARIS_THREADS || USE_WINDOWS_THREADS) /* Provide dummy implementation if threads are not supported. */ # define gl_thread_yield() 0 #endif /* ========================================================================= */ #endif /* _GLTHREAD_YIELD_H */ gnuastro-0.2.33-8a3b/bootstrapped/tests/glthread/thread.c0000644000175000017500000001427313004436755020210 00000000000000/* Creating and controlling threads. Copyright (C) 2005-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible , 2005. Based on GCC's gthr-posix.h, gthr-posix95.h, gthr-solaris.h, gthr-win32.h. */ #include /* Specification. */ # define _GLTHREAD_THREAD_INLINE _GL_EXTERN_INLINE #include "glthread/thread.h" #include #include "glthread/lock.h" /* ========================================================================= */ #if USE_POSIX_THREADS #include #if defined PTW32_VERSION || defined __MVS__ const gl_thread_t gl_null_thread /* = { .p = NULL } */; #endif #endif /* ========================================================================= */ #if USE_WINDOWS_THREADS #include /* -------------------------- gl_thread_t datatype -------------------------- */ /* The Thread-Local Storage (TLS) key that allows to access each thread's 'struct gl_thread_struct *' pointer. */ static DWORD self_key = (DWORD)-1; /* Initializes self_key. This function must only be called once. */ static void do_init_self_key (void) { self_key = TlsAlloc (); /* If this fails, we're hosed. */ if (self_key == (DWORD)-1) abort (); } /* Initializes self_key. */ static void init_self_key (void) { gl_once_define(static, once) gl_once (once, do_init_self_key); } /* This structure contains information about a thread. It is stored in TLS under key self_key. */ struct gl_thread_struct { /* Fields for managing the handle. */ HANDLE volatile handle; CRITICAL_SECTION handle_lock; /* Fields for managing the exit value. */ void * volatile result; /* Fields for managing the thread start. */ void * (*func) (void *); void *arg; }; /* Return a real HANDLE object for the current thread. */ static HANDLE get_current_thread_handle (void) { HANDLE this_handle; /* GetCurrentThread() returns a pseudo-handle, i.e. only a symbolic identifier, not a real handle. */ if (!DuplicateHandle (GetCurrentProcess (), GetCurrentThread (), GetCurrentProcess (), &this_handle, 0, FALSE, DUPLICATE_SAME_ACCESS)) abort (); return this_handle; } gl_thread_t gl_thread_self_func (void) { gl_thread_t thread; if (self_key == (DWORD)-1) init_self_key (); thread = TlsGetValue (self_key); if (thread == NULL) { /* This happens only in threads that have not been created through glthread_create(), such as the main thread. */ for (;;) { thread = (struct gl_thread_struct *) malloc (sizeof (struct gl_thread_struct)); if (thread != NULL) break; /* Memory allocation failed. There is not much we can do. Have to busy-loop, waiting for the availability of memory. */ Sleep (1); } thread->handle = get_current_thread_handle (); InitializeCriticalSection (&thread->handle_lock); thread->result = NULL; /* just to be deterministic */ TlsSetValue (self_key, thread); } return thread; } /* The main function of a freshly creating thread. It's a wrapper around the FUNC and ARG arguments passed to glthread_create_func. */ static unsigned int WINAPI wrapper_func (void *varg) { struct gl_thread_struct *thread = (struct gl_thread_struct *)varg; EnterCriticalSection (&thread->handle_lock); /* Create a new handle for the thread only if the parent thread did not yet fill in the handle. */ if (thread->handle == NULL) thread->handle = get_current_thread_handle (); LeaveCriticalSection (&thread->handle_lock); if (self_key == (DWORD)-1) init_self_key (); TlsSetValue (self_key, thread); /* Run the thread. Store the exit value if the thread was not terminated otherwise. */ thread->result = thread->func (thread->arg); return 0; } int glthread_create_func (gl_thread_t *threadp, void * (*func) (void *), void *arg) { struct gl_thread_struct *thread = (struct gl_thread_struct *) malloc (sizeof (struct gl_thread_struct)); if (thread == NULL) return ENOMEM; thread->handle = NULL; InitializeCriticalSection (&thread->handle_lock); thread->result = NULL; /* just to be deterministic */ thread->func = func; thread->arg = arg; { unsigned int thread_id; HANDLE thread_handle; thread_handle = (HANDLE) _beginthreadex (NULL, 100000, wrapper_func, thread, 0, &thread_id); /* calls CreateThread with the same arguments */ if (thread_handle == NULL) { DeleteCriticalSection (&thread->handle_lock); free (thread); return EAGAIN; } EnterCriticalSection (&thread->handle_lock); if (thread->handle == NULL) thread->handle = thread_handle; else /* thread->handle was already set by the thread itself. */ CloseHandle (thread_handle); LeaveCriticalSection (&thread->handle_lock); *threadp = thread; return 0; } } int glthread_join_func (gl_thread_t thread, void **retvalp) { if (thread == NULL) return EINVAL; if (thread == gl_thread_self ()) return EDEADLK; if (WaitForSingleObject (thread->handle, INFINITE) == WAIT_FAILED) return EINVAL; if (retvalp != NULL) *retvalp = thread->result; DeleteCriticalSection (&thread->handle_lock); CloseHandle (thread->handle); free (thread); return 0; } int gl_thread_exit_func (void *retval) { gl_thread_t thread = gl_thread_self (); thread->result = retval; _endthreadex (0); /* calls ExitThread (0) */ abort (); } #endif /* ========================================================================= */ gnuastro-0.2.33-8a3b/bootstrapped/tests/glthread/thread.h0000644000175000017500000003234713004436755020217 00000000000000/* Creating and controlling threads. Copyright (C) 2005-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible , 2005. Based on GCC's gthr-posix.h, gthr-posix95.h, gthr-solaris.h, gthr-win32.h. */ /* This file contains primitives for creating and controlling threads. Thread data type: gl_thread_t. Creating a thread: thread = gl_thread_create (func, arg); Or with control of error handling: err = glthread_create (&thread, func, arg); extern int glthread_create (gl_thread_t *result, void *(*func) (void *), void *arg); Querying and changing the signal mask of a thread (not supported on all platforms): gl_thread_sigmask (how, newmask, oldmask); Or with control of error handling: err = glthread_sigmask (how, newmask, oldmask); extern int glthread_sigmask (int how, const sigset_t *newmask, sigset_t *oldmask); Waiting for termination of another thread: gl_thread_join (thread, &return_value); Or with control of error handling: err = glthread_join (thread, &return_value); extern int glthread_join (gl_thread_t thread, void **return_value_ptr); Getting a reference to the current thread: current = gl_thread_self (); extern gl_thread_t gl_thread_self (void); Getting a reference to the current thread as a pointer, for debugging: ptr = gl_thread_self_pointer (); extern void * gl_thread_self_pointer (void); Terminating the current thread: gl_thread_exit (return_value); extern _Noreturn void gl_thread_exit (void *return_value); Requesting custom code to be executed at fork() time(not supported on all platforms): gl_thread_atfork (prepare_func, parent_func, child_func); Or with control of error handling: err = glthread_atfork (prepare_func, parent_func, child_func); extern int glthread_atfork (void (*prepare_func) (void), void (*parent_func) (void), void (*child_func) (void)); Note that even on platforms where this is supported, use of fork() and threads together is problematic, see */ #ifndef _GLTHREAD_THREAD_H #define _GLTHREAD_THREAD_H #include #include #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef _GLTHREAD_THREAD_INLINE # define _GLTHREAD_THREAD_INLINE _GL_INLINE #endif /* ========================================================================= */ #if USE_POSIX_THREADS /* Use the POSIX threads library. */ # include # ifdef __cplusplus extern "C" { # endif # if PTHREAD_IN_USE_DETECTION_HARD /* The pthread_in_use() detection needs to be done at runtime. */ # define pthread_in_use() \ glthread_in_use () extern int glthread_in_use (void); # endif # if USE_POSIX_THREADS_WEAK /* Use weak references to the POSIX threads library. */ /* Weak references avoid dragging in external libraries if the other parts of the program don't use them. Here we use them, because we don't want every program that uses libintl to depend on libpthread. This assumes that libpthread would not be loaded after libintl; i.e. if libintl is loaded first, by an executable that does not depend on libpthread, and then a module is dynamically loaded that depends on libpthread, libintl will not be multithread-safe. */ /* The way to test at runtime whether libpthread is present is to test whether a function pointer's value, such as &pthread_mutex_init, is non-NULL. However, some versions of GCC have a bug through which, in PIC mode, &foo != NULL always evaluates to true if there is a direct call to foo(...) in the same function. To avoid this, we test the address of a function in libpthread that we don't use. */ # pragma weak pthread_create # ifdef __clang__ /* Without this, clang complains that pthread_sigmask is never declared. */ # include # endif # pragma weak pthread_sigmask # pragma weak pthread_join # ifndef pthread_self # pragma weak pthread_self # endif # pragma weak pthread_exit # if HAVE_PTHREAD_ATFORK # pragma weak pthread_atfork # endif # if !PTHREAD_IN_USE_DETECTION_HARD # pragma weak pthread_cancel # define pthread_in_use() (pthread_cancel != NULL) # endif # else # if !PTHREAD_IN_USE_DETECTION_HARD # define pthread_in_use() 1 # endif # endif /* -------------------------- gl_thread_t datatype -------------------------- */ /* This choice of gl_thread_t assumes that pthread_equal (a, b) is equivalent to ((a) == (b)). This is the case on all platforms in use in 2008. */ typedef pthread_t gl_thread_t; # define glthread_create(THREADP, FUNC, ARG) \ (pthread_in_use () ? pthread_create (THREADP, NULL, FUNC, ARG) : ENOSYS) # define glthread_sigmask(HOW, SET, OSET) \ (pthread_in_use () ? pthread_sigmask (HOW, SET, OSET) : 0) # define glthread_join(THREAD, RETVALP) \ (pthread_in_use () ? pthread_join (THREAD, RETVALP) : 0) # ifdef PTW32_VERSION /* In pthreads-win32, pthread_t is a struct with a pointer field 'p' and other fields. */ # define gl_thread_self() \ (pthread_in_use () ? pthread_self () : gl_null_thread) # define gl_thread_self_pointer() \ (pthread_in_use () ? pthread_self ().p : NULL) extern const gl_thread_t gl_null_thread; # elif defined __MVS__ /* On IBM z/OS, pthread_t is a struct with an 8-byte '__' field. The first three bytes of this field appear to uniquely identify a pthread_t, though not necessarily representing a pointer. */ # define gl_thread_self() \ (pthread_in_use () ? pthread_self () : gl_null_thread) # define gl_thread_self_pointer() \ (pthread_in_use () ? *((void **) pthread_self ().__) : NULL) extern const gl_thread_t gl_null_thread; # else # define gl_thread_self() \ (pthread_in_use () ? pthread_self () : (pthread_t) NULL) # define gl_thread_self_pointer() \ (pthread_in_use () ? (void *) pthread_self () : NULL) # endif # define gl_thread_exit(RETVAL) \ (pthread_in_use () ? pthread_exit (RETVAL) : 0) # if HAVE_PTHREAD_ATFORK # define glthread_atfork(PREPARE_FUNC, PARENT_FUNC, CHILD_FUNC) \ (pthread_in_use () ? pthread_atfork (PREPARE_FUNC, PARENT_FUNC, CHILD_FUNC) : 0) # else # define glthread_atfork(PREPARE_FUNC, PARENT_FUNC, CHILD_FUNC) 0 # endif # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_PTH_THREADS /* Use the GNU Pth threads library. */ # include # ifdef __cplusplus extern "C" { # endif # if USE_PTH_THREADS_WEAK /* Use weak references to the GNU Pth threads library. */ # pragma weak pth_spawn # pragma weak pth_sigmask # pragma weak pth_join # pragma weak pth_self # pragma weak pth_exit # pragma weak pth_cancel # define pth_in_use() (pth_cancel != NULL) # else # define pth_in_use() 1 # endif /* -------------------------- gl_thread_t datatype -------------------------- */ typedef pth_t gl_thread_t; # define glthread_create(THREADP, FUNC, ARG) \ (pth_in_use () ? ((*(THREADP) = pth_spawn (NULL, FUNC, ARG)) ? 0 : errno) : 0) # define glthread_sigmask(HOW, SET, OSET) \ (pth_in_use () && !pth_sigmask (HOW, SET, OSET) ? errno : 0) # define glthread_join(THREAD, RETVALP) \ (pth_in_use () && !pth_join (THREAD, RETVALP) ? errno : 0) # define gl_thread_self() \ (pth_in_use () ? (void *) pth_self () : NULL) # define gl_thread_self_pointer() \ gl_thread_self () # define gl_thread_exit(RETVAL) \ (pth_in_use () ? pth_exit (RETVAL) : 0) # define glthread_atfork(PREPARE_FUNC, PARENT_FUNC, CHILD_FUNC) 0 # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_SOLARIS_THREADS /* Use the old Solaris threads library. */ # include # include # ifdef __cplusplus extern "C" { # endif # if USE_SOLARIS_THREADS_WEAK /* Use weak references to the old Solaris threads library. */ # pragma weak thr_create # pragma weak thr_join # pragma weak thr_self # pragma weak thr_exit # pragma weak thr_suspend # define thread_in_use() (thr_suspend != NULL) # else # define thread_in_use() 1 # endif /* -------------------------- gl_thread_t datatype -------------------------- */ typedef thread_t gl_thread_t; # define glthread_create(THREADP, FUNC, ARG) \ (thread_in_use () ? thr_create (NULL, 0, FUNC, ARG, 0, THREADP) : 0) # define glthread_sigmask(HOW, SET, OSET) \ (thread_in_use () ? sigprocmask (HOW, SET, OSET) : 0) # define glthread_join(THREAD, RETVALP) \ (thread_in_use () ? thr_join (THREAD, NULL, RETVALP) : 0) # define gl_thread_self() \ (thread_in_use () ? (void *) thr_self () : NULL) # define gl_thread_self_pointer() \ gl_thread_self () # define gl_thread_exit(RETVAL) \ (thread_in_use () ? thr_exit (RETVAL) : 0) # define glthread_atfork(PREPARE_FUNC, PARENT_FUNC, CHILD_FUNC) 0 # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_WINDOWS_THREADS # define WIN32_LEAN_AND_MEAN /* avoid including junk */ # include # ifdef __cplusplus extern "C" { # endif /* -------------------------- gl_thread_t datatype -------------------------- */ /* The gl_thread_t is a pointer to a structure in memory. Why not the thread handle? If it were the thread handle, it would be hard to implement gl_thread_self() (since GetCurrentThread () returns a pseudo- handle, DuplicateHandle (GetCurrentThread ()) returns a handle that must be closed afterwards, and there is no function for quickly retrieving a thread handle from its id). Why not the thread id? I tried it. It did not work: Sometimes ids appeared that did not belong to running threads, and glthread_join failed with ESRCH. */ typedef struct gl_thread_struct *gl_thread_t; # define glthread_create(THREADP, FUNC, ARG) \ glthread_create_func (THREADP, FUNC, ARG) # define glthread_sigmask(HOW, SET, OSET) \ /* unsupported */ 0 # define glthread_join(THREAD, RETVALP) \ glthread_join_func (THREAD, RETVALP) # define gl_thread_self() \ gl_thread_self_func () # define gl_thread_self_pointer() \ gl_thread_self () # define gl_thread_exit(RETVAL) \ gl_thread_exit_func (RETVAL) # define glthread_atfork(PREPARE_FUNC, PARENT_FUNC, CHILD_FUNC) 0 extern int glthread_create_func (gl_thread_t *threadp, void * (*func) (void *), void *arg); extern int glthread_join_func (gl_thread_t thread, void **retvalp); extern gl_thread_t gl_thread_self_func (void); extern int gl_thread_exit_func (void *retval); # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if !(USE_POSIX_THREADS || USE_PTH_THREADS || USE_SOLARIS_THREADS || USE_WINDOWS_THREADS) /* Provide dummy implementation if threads are not supported. */ typedef int gl_thread_t; # define glthread_create(THREADP, FUNC, ARG) ENOSYS # define glthread_sigmask(HOW, SET, OSET) 0 # define glthread_join(THREAD, RETVALP) 0 # define gl_thread_self() 0 # define gl_thread_self_pointer() \ ((void *) gl_thread_self ()) # define gl_thread_exit(RETVAL) 0 # define glthread_atfork(PREPARE_FUNC, PARENT_FUNC, CHILD_FUNC) 0 #endif /* ========================================================================= */ /* Macros with built-in error handling. */ #ifdef __cplusplus extern "C" { #endif _GLTHREAD_THREAD_INLINE gl_thread_t gl_thread_create (void *(*func) (void *arg), void *arg) { gl_thread_t thread; int ret; ret = glthread_create (&thread, func, arg); if (ret != 0) abort (); return thread; } #define gl_thread_sigmask(HOW, SET, OSET) \ do \ { \ if (glthread_sigmask (HOW, SET, OSET)) \ abort (); \ } \ while (0) #define gl_thread_join(THREAD, RETVAL) \ do \ { \ if (glthread_join (THREAD, RETVAL)) \ abort (); \ } \ while (0) #define gl_thread_atfork(PREPARE, PARENT, CHILD) \ do \ { \ if (glthread_atfork (PREPARE, PARENT, CHILD)) \ abort (); \ } \ while (0) #ifdef __cplusplus } #endif _GL_INLINE_HEADER_END #endif /* _GLTHREAD_THREAD_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/0000755000175000017500000000000013004464723014454 500000000000000gnuastro-0.2.33-8a3b/bootstrapped/lib/wctype.in.h0000644000175000017500000003263213004436754016476 00000000000000/* A substitute for ISO C99 , for platforms that lack it. Copyright (C) 2006-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible and Paul Eggert. */ /* * ISO C 99 for platforms that lack it. * * * iswctype, towctrans, towlower, towupper, wctrans, wctype, * wctrans_t, and wctype_t are not yet implemented. */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if (defined __MINGW32__ && defined __CTYPE_H_SOURCED__) /* Special invocation convention: - With MinGW 3.22, when includes , only some part of is being processed, which doesn't include the idempotency guard. */ #@INCLUDE_NEXT@ @NEXT_WCTYPE_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_WCTYPE_H #if @HAVE_WINT_T@ /* Solaris 2.5 has a bug: must be included before . Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ # include # include # include # include #endif /* mingw has declarations of towupper and towlower in as well . Include in advance to avoid rpl_ prefix being added to the declarations. */ #ifdef __MINGW32__ # include #endif /* Include the original if it exists. BeOS 5 has the functions but no . */ /* The include_next requires a split double-inclusion guard. */ #if @HAVE_WCTYPE_H@ # @INCLUDE_NEXT@ @NEXT_WCTYPE_H@ #endif #ifndef _@GUARD_PREFIX@_WCTYPE_H #define _@GUARD_PREFIX@_WCTYPE_H #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef _GL_WCTYPE_INLINE # define _GL_WCTYPE_INLINE _GL_INLINE #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Solaris 2.6 includes which includes which #defines a number of identifiers in the application namespace. Revert these #defines. */ #ifdef __sun # undef multibyte # undef eucw1 # undef eucw2 # undef eucw3 # undef scrw1 # undef scrw2 # undef scrw3 #endif /* Define wint_t and WEOF. (Also done in wchar.in.h.) */ #if !@HAVE_WINT_T@ && !defined wint_t # define wint_t int # ifndef WEOF # define WEOF -1 # endif #else /* MSVC defines wint_t as 'unsigned short' in . This is too small: ISO C 99 section 7.24.1.(2) says that wint_t must be "unchanged by default argument promotions". Override it. */ # if defined _MSC_VER # if !GNULIB_defined_wint_t # include typedef unsigned int rpl_wint_t; # undef wint_t # define wint_t rpl_wint_t # define GNULIB_defined_wint_t 1 # endif # endif # ifndef WEOF # define WEOF ((wint_t) -1) # endif #endif #if !GNULIB_defined_wctype_functions /* FreeBSD 4.4 to 4.11 has but lacks the functions. Linux libc5 has and the functions but they are broken. Assume all 11 functions (all isw* except iswblank) are implemented the same way, or not at all. */ # if ! @HAVE_ISWCNTRL@ || @REPLACE_ISWCNTRL@ /* IRIX 5.3 has macros but no functions, its isw* macros refer to an undefined variable _ctmp_ and to macros like _P, and they refer to system functions like _iswctype that are not in the standard C library. Rather than try to get ancient buggy implementations like this to work, just disable them. */ # undef iswalnum # undef iswalpha # undef iswblank # undef iswcntrl # undef iswdigit # undef iswgraph # undef iswlower # undef iswprint # undef iswpunct # undef iswspace # undef iswupper # undef iswxdigit # undef towlower # undef towupper /* Linux libc5 has and the functions but they are broken. */ # if @REPLACE_ISWCNTRL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define iswalnum rpl_iswalnum # define iswalpha rpl_iswalpha # define iswblank rpl_iswblank # define iswcntrl rpl_iswcntrl # define iswdigit rpl_iswdigit # define iswgraph rpl_iswgraph # define iswlower rpl_iswlower # define iswprint rpl_iswprint # define iswpunct rpl_iswpunct # define iswspace rpl_iswspace # define iswupper rpl_iswupper # define iswxdigit rpl_iswxdigit # endif # endif # if @REPLACE_TOWLOWER@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define towlower rpl_towlower # define towupper rpl_towupper # endif # endif _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswalnum # else iswalnum # endif (wint_t wc) { return ((wc >= '0' && wc <= '9') || ((wc & ~0x20) >= 'A' && (wc & ~0x20) <= 'Z')); } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswalpha # else iswalpha # endif (wint_t wc) { return (wc & ~0x20) >= 'A' && (wc & ~0x20) <= 'Z'; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswblank # else iswblank # endif (wint_t wc) { return wc == ' ' || wc == '\t'; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswcntrl # else iswcntrl # endif (wint_t wc) { return (wc & ~0x1f) == 0 || wc == 0x7f; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswdigit # else iswdigit # endif (wint_t wc) { return wc >= '0' && wc <= '9'; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswgraph # else iswgraph # endif (wint_t wc) { return wc >= '!' && wc <= '~'; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswlower # else iswlower # endif (wint_t wc) { return wc >= 'a' && wc <= 'z'; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswprint # else iswprint # endif (wint_t wc) { return wc >= ' ' && wc <= '~'; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswpunct # else iswpunct # endif (wint_t wc) { return (wc >= '!' && wc <= '~' && !((wc >= '0' && wc <= '9') || ((wc & ~0x20) >= 'A' && (wc & ~0x20) <= 'Z'))); } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswspace # else iswspace # endif (wint_t wc) { return (wc == ' ' || wc == '\t' || wc == '\n' || wc == '\v' || wc == '\f' || wc == '\r'); } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswupper # else iswupper # endif (wint_t wc) { return wc >= 'A' && wc <= 'Z'; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswxdigit # else iswxdigit # endif (wint_t wc) { return ((wc >= '0' && wc <= '9') || ((wc & ~0x20) >= 'A' && (wc & ~0x20) <= 'F')); } _GL_WCTYPE_INLINE wint_t # if @REPLACE_TOWLOWER@ rpl_towlower # else towlower # endif (wint_t wc) { return (wc >= 'A' && wc <= 'Z' ? wc - 'A' + 'a' : wc); } _GL_WCTYPE_INLINE wint_t # if @REPLACE_TOWLOWER@ rpl_towupper # else towupper # endif (wint_t wc) { return (wc >= 'a' && wc <= 'z' ? wc - 'a' + 'A' : wc); } # elif @GNULIB_ISWBLANK@ && (! @HAVE_ISWBLANK@ || @REPLACE_ISWBLANK@) /* Only the iswblank function is missing. */ # if @REPLACE_ISWBLANK@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define iswblank rpl_iswblank # endif _GL_FUNCDECL_RPL (iswblank, int, (wint_t wc)); # else _GL_FUNCDECL_SYS (iswblank, int, (wint_t wc)); # endif # endif # if defined __MINGW32__ /* On native Windows, wchar_t is uint16_t, and wint_t is uint32_t. The functions towlower and towupper are implemented in the MSVCRT library to take a wchar_t argument and return a wchar_t result. mingw declares these functions to take a wint_t argument and return a wint_t result. This means that: 1. When the user passes an argument outside the range 0x0000..0xFFFF, the function will look only at the lower 16 bits. This is allowed according to POSIX. 2. The return value is returned in the lower 16 bits of the result register. The upper 16 bits are random: whatever happened to be in that part of the result register. We need to fix this by adding a zero-extend from wchar_t to wint_t after the call. */ _GL_WCTYPE_INLINE wint_t rpl_towlower (wint_t wc) { return (wint_t) (wchar_t) towlower (wc); } # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define towlower rpl_towlower # endif _GL_WCTYPE_INLINE wint_t rpl_towupper (wint_t wc) { return (wint_t) (wchar_t) towupper (wc); } # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define towupper rpl_towupper # endif # endif /* __MINGW32__ */ # define GNULIB_defined_wctype_functions 1 #endif #if @REPLACE_ISWCNTRL@ _GL_CXXALIAS_RPL (iswalnum, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswalpha, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswcntrl, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswdigit, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswgraph, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswlower, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswprint, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswpunct, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswspace, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswupper, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswxdigit, int, (wint_t wc)); #else _GL_CXXALIAS_SYS (iswalnum, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswalpha, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswcntrl, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswdigit, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswgraph, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswlower, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswprint, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswpunct, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswspace, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswupper, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswxdigit, int, (wint_t wc)); #endif _GL_CXXALIASWARN (iswalnum); _GL_CXXALIASWARN (iswalpha); _GL_CXXALIASWARN (iswcntrl); _GL_CXXALIASWARN (iswdigit); _GL_CXXALIASWARN (iswgraph); _GL_CXXALIASWARN (iswlower); _GL_CXXALIASWARN (iswprint); _GL_CXXALIASWARN (iswpunct); _GL_CXXALIASWARN (iswspace); _GL_CXXALIASWARN (iswupper); _GL_CXXALIASWARN (iswxdigit); #if @GNULIB_ISWBLANK@ # if @REPLACE_ISWCNTRL@ || @REPLACE_ISWBLANK@ _GL_CXXALIAS_RPL (iswblank, int, (wint_t wc)); # else _GL_CXXALIAS_SYS (iswblank, int, (wint_t wc)); # endif _GL_CXXALIASWARN (iswblank); #endif #if !@HAVE_WCTYPE_T@ # if !GNULIB_defined_wctype_t typedef void * wctype_t; # define GNULIB_defined_wctype_t 1 # endif #endif /* Get a descriptor for a wide character property. */ #if @GNULIB_WCTYPE@ # if !@HAVE_WCTYPE_T@ _GL_FUNCDECL_SYS (wctype, wctype_t, (const char *name)); # endif _GL_CXXALIAS_SYS (wctype, wctype_t, (const char *name)); _GL_CXXALIASWARN (wctype); #elif defined GNULIB_POSIXCHECK # undef wctype # if HAVE_RAW_DECL_WCTYPE _GL_WARN_ON_USE (wctype, "wctype is unportable - " "use gnulib module wctype for portability"); # endif #endif /* Test whether a wide character has a given property. The argument WC must be either a wchar_t value or WEOF. The argument DESC must have been returned by the wctype() function. */ #if @GNULIB_ISWCTYPE@ # if !@HAVE_WCTYPE_T@ _GL_FUNCDECL_SYS (iswctype, int, (wint_t wc, wctype_t desc)); # endif _GL_CXXALIAS_SYS (iswctype, int, (wint_t wc, wctype_t desc)); _GL_CXXALIASWARN (iswctype); #elif defined GNULIB_POSIXCHECK # undef iswctype # if HAVE_RAW_DECL_ISWCTYPE _GL_WARN_ON_USE (iswctype, "iswctype is unportable - " "use gnulib module iswctype for portability"); # endif #endif #if @REPLACE_TOWLOWER@ || defined __MINGW32__ _GL_CXXALIAS_RPL (towlower, wint_t, (wint_t wc)); _GL_CXXALIAS_RPL (towupper, wint_t, (wint_t wc)); #else _GL_CXXALIAS_SYS (towlower, wint_t, (wint_t wc)); _GL_CXXALIAS_SYS (towupper, wint_t, (wint_t wc)); #endif _GL_CXXALIASWARN (towlower); _GL_CXXALIASWARN (towupper); #if !@HAVE_WCTRANS_T@ # if !GNULIB_defined_wctrans_t typedef void * wctrans_t; # define GNULIB_defined_wctrans_t 1 # endif #endif /* Get a descriptor for a wide character case conversion. */ #if @GNULIB_WCTRANS@ # if !@HAVE_WCTRANS_T@ _GL_FUNCDECL_SYS (wctrans, wctrans_t, (const char *name)); # endif _GL_CXXALIAS_SYS (wctrans, wctrans_t, (const char *name)); _GL_CXXALIASWARN (wctrans); #elif defined GNULIB_POSIXCHECK # undef wctrans # if HAVE_RAW_DECL_WCTRANS _GL_WARN_ON_USE (wctrans, "wctrans is unportable - " "use gnulib module wctrans for portability"); # endif #endif /* Perform a given case conversion on a wide character. The argument WC must be either a wchar_t value or WEOF. The argument DESC must have been returned by the wctrans() function. */ #if @GNULIB_TOWCTRANS@ # if !@HAVE_WCTRANS_T@ _GL_FUNCDECL_SYS (towctrans, wint_t, (wint_t wc, wctrans_t desc)); # endif _GL_CXXALIAS_SYS (towctrans, wint_t, (wint_t wc, wctrans_t desc)); _GL_CXXALIASWARN (towctrans); #elif defined GNULIB_POSIXCHECK # undef towctrans # if HAVE_RAW_DECL_TOWCTRANS _GL_WARN_ON_USE (towctrans, "towctrans is unportable - " "use gnulib module towctrans for portability"); # endif #endif _GL_INLINE_HEADER_END #endif /* _@GUARD_PREFIX@_WCTYPE_H */ #endif /* _@GUARD_PREFIX@_WCTYPE_H */ #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/wchar.in.h0000644000175000017500000010313113004436754016260 00000000000000/* A substitute for ISO C99 , for platforms that have issues. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Eric Blake. */ /* * ISO C 99 for platforms that have issues. * * * For now, this just ensures proper prerequisite inclusion order and * the declaration of wcwidth(). */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if (((defined __need_mbstate_t || defined __need_wint_t) \ && !defined __MINGW32__ && !defined __KLIBC__) \ || (defined __hpux \ && ((defined _INTTYPES_INCLUDED && !defined strtoimax) \ || defined _GL_JUST_INCLUDE_SYSTEM_WCHAR_H)) \ || (defined __MINGW32__ && defined __STRING_H_SOURCED__) \ || defined _GL_ALREADY_INCLUDING_WCHAR_H) /* Special invocation convention: - Inside glibc and uClibc header files, but not MinGW. - On HP-UX 11.00 we have a sequence of nested includes -> -> , and the latter includes , once indirectly -> -> -> and once directly. In both situations 'wint_t' is not yet defined, therefore we cannot provide the function overrides; instead include only the system's . - With MinGW 3.22, when includes , only some part of is actually processed, and that doesn't include 'mbstate_t'. - On IRIX 6.5, similarly, we have an include -> , and the latter includes . But here, we have no way to detect whether is completely included or is still being included. */ #@INCLUDE_NEXT@ @NEXT_WCHAR_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_WCHAR_H #define _GL_ALREADY_INCLUDING_WCHAR_H #if @HAVE_FEATURES_H@ # include /* for __GLIBC__ */ #endif /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . In some builds of uClibc, is nonexistent and wchar_t is defined by . But avoid namespace pollution on glibc systems. */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include #endif #ifndef __GLIBC__ # include # include #endif /* Include the original if it exists. Some builds of uClibc lack it. */ /* The include_next requires a split double-inclusion guard. */ #if @HAVE_WCHAR_H@ # @INCLUDE_NEXT@ @NEXT_WCHAR_H@ #endif #undef _GL_ALREADY_INCLUDING_WCHAR_H #ifndef _@GUARD_PREFIX@_WCHAR_H #define _@GUARD_PREFIX@_WCHAR_H /* The __attribute__ feature is available in gcc versions 2.5 and later. The attribute __pure__ was added in gcc 2.96. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 96) # define _GL_ATTRIBUTE_PURE __attribute__ ((__pure__)) #else # define _GL_ATTRIBUTE_PURE /* empty */ #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Define wint_t and WEOF. (Also done in wctype.in.h.) */ #if !@HAVE_WINT_T@ && !defined wint_t # define wint_t int # ifndef WEOF # define WEOF -1 # endif #else /* MSVC defines wint_t as 'unsigned short' in . This is too small: ISO C 99 section 7.24.1.(2) says that wint_t must be "unchanged by default argument promotions". Override it. */ # if defined _MSC_VER # if !GNULIB_defined_wint_t # include typedef unsigned int rpl_wint_t; # undef wint_t # define wint_t rpl_wint_t # define GNULIB_defined_wint_t 1 # endif # endif # ifndef WEOF # define WEOF ((wint_t) -1) # endif #endif /* Override mbstate_t if it is too small. On IRIX 6.5, sizeof (mbstate_t) == 1, which is not sufficient for implementing mbrtowc for encodings like UTF-8. */ #if !(@HAVE_MBSINIT@ && @HAVE_MBRTOWC@) || @REPLACE_MBSTATE_T@ # if !GNULIB_defined_mbstate_t typedef int rpl_mbstate_t; # undef mbstate_t # define mbstate_t rpl_mbstate_t # define GNULIB_defined_mbstate_t 1 # endif #endif /* Convert a single-byte character to a wide character. */ #if @GNULIB_BTOWC@ # if @REPLACE_BTOWC@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef btowc # define btowc rpl_btowc # endif _GL_FUNCDECL_RPL (btowc, wint_t, (int c) _GL_ATTRIBUTE_PURE); _GL_CXXALIAS_RPL (btowc, wint_t, (int c)); # else # if !@HAVE_BTOWC@ _GL_FUNCDECL_SYS (btowc, wint_t, (int c) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (btowc, wint_t, (int c)); # endif _GL_CXXALIASWARN (btowc); #elif defined GNULIB_POSIXCHECK # undef btowc # if HAVE_RAW_DECL_BTOWC _GL_WARN_ON_USE (btowc, "btowc is unportable - " "use gnulib module btowc for portability"); # endif #endif /* Convert a wide character to a single-byte character. */ #if @GNULIB_WCTOB@ # if @REPLACE_WCTOB@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef wctob # define wctob rpl_wctob # endif _GL_FUNCDECL_RPL (wctob, int, (wint_t wc) _GL_ATTRIBUTE_PURE); _GL_CXXALIAS_RPL (wctob, int, (wint_t wc)); # else # if !defined wctob && !@HAVE_DECL_WCTOB@ /* wctob is provided by gnulib, or wctob exists but is not declared. */ _GL_FUNCDECL_SYS (wctob, int, (wint_t wc) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wctob, int, (wint_t wc)); # endif _GL_CXXALIASWARN (wctob); #elif defined GNULIB_POSIXCHECK # undef wctob # if HAVE_RAW_DECL_WCTOB _GL_WARN_ON_USE (wctob, "wctob is unportable - " "use gnulib module wctob for portability"); # endif #endif /* Test whether *PS is in the initial state. */ #if @GNULIB_MBSINIT@ # if @REPLACE_MBSINIT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mbsinit # define mbsinit rpl_mbsinit # endif _GL_FUNCDECL_RPL (mbsinit, int, (const mbstate_t *ps)); _GL_CXXALIAS_RPL (mbsinit, int, (const mbstate_t *ps)); # else # if !@HAVE_MBSINIT@ _GL_FUNCDECL_SYS (mbsinit, int, (const mbstate_t *ps)); # endif _GL_CXXALIAS_SYS (mbsinit, int, (const mbstate_t *ps)); # endif _GL_CXXALIASWARN (mbsinit); #elif defined GNULIB_POSIXCHECK # undef mbsinit # if HAVE_RAW_DECL_MBSINIT _GL_WARN_ON_USE (mbsinit, "mbsinit is unportable - " "use gnulib module mbsinit for portability"); # endif #endif /* Convert a multibyte character to a wide character. */ #if @GNULIB_MBRTOWC@ # if @REPLACE_MBRTOWC@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mbrtowc # define mbrtowc rpl_mbrtowc # endif _GL_FUNCDECL_RPL (mbrtowc, size_t, (wchar_t *pwc, const char *s, size_t n, mbstate_t *ps)); _GL_CXXALIAS_RPL (mbrtowc, size_t, (wchar_t *pwc, const char *s, size_t n, mbstate_t *ps)); # else # if !@HAVE_MBRTOWC@ _GL_FUNCDECL_SYS (mbrtowc, size_t, (wchar_t *pwc, const char *s, size_t n, mbstate_t *ps)); # endif _GL_CXXALIAS_SYS (mbrtowc, size_t, (wchar_t *pwc, const char *s, size_t n, mbstate_t *ps)); # endif _GL_CXXALIASWARN (mbrtowc); #elif defined GNULIB_POSIXCHECK # undef mbrtowc # if HAVE_RAW_DECL_MBRTOWC _GL_WARN_ON_USE (mbrtowc, "mbrtowc is unportable - " "use gnulib module mbrtowc for portability"); # endif #endif /* Recognize a multibyte character. */ #if @GNULIB_MBRLEN@ # if @REPLACE_MBRLEN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mbrlen # define mbrlen rpl_mbrlen # endif _GL_FUNCDECL_RPL (mbrlen, size_t, (const char *s, size_t n, mbstate_t *ps)); _GL_CXXALIAS_RPL (mbrlen, size_t, (const char *s, size_t n, mbstate_t *ps)); # else # if !@HAVE_MBRLEN@ _GL_FUNCDECL_SYS (mbrlen, size_t, (const char *s, size_t n, mbstate_t *ps)); # endif _GL_CXXALIAS_SYS (mbrlen, size_t, (const char *s, size_t n, mbstate_t *ps)); # endif _GL_CXXALIASWARN (mbrlen); #elif defined GNULIB_POSIXCHECK # undef mbrlen # if HAVE_RAW_DECL_MBRLEN _GL_WARN_ON_USE (mbrlen, "mbrlen is unportable - " "use gnulib module mbrlen for portability"); # endif #endif /* Convert a string to a wide string. */ #if @GNULIB_MBSRTOWCS@ # if @REPLACE_MBSRTOWCS@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mbsrtowcs # define mbsrtowcs rpl_mbsrtowcs # endif _GL_FUNCDECL_RPL (mbsrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (mbsrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t len, mbstate_t *ps)); # else # if !@HAVE_MBSRTOWCS@ _GL_FUNCDECL_SYS (mbsrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (mbsrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t len, mbstate_t *ps)); # endif _GL_CXXALIASWARN (mbsrtowcs); #elif defined GNULIB_POSIXCHECK # undef mbsrtowcs # if HAVE_RAW_DECL_MBSRTOWCS _GL_WARN_ON_USE (mbsrtowcs, "mbsrtowcs is unportable - " "use gnulib module mbsrtowcs for portability"); # endif #endif /* Convert a string to a wide string. */ #if @GNULIB_MBSNRTOWCS@ # if @REPLACE_MBSNRTOWCS@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mbsnrtowcs # define mbsnrtowcs rpl_mbsnrtowcs # endif _GL_FUNCDECL_RPL (mbsnrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t srclen, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (mbsnrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t srclen, size_t len, mbstate_t *ps)); # else # if !@HAVE_MBSNRTOWCS@ _GL_FUNCDECL_SYS (mbsnrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t srclen, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (mbsnrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t srclen, size_t len, mbstate_t *ps)); # endif _GL_CXXALIASWARN (mbsnrtowcs); #elif defined GNULIB_POSIXCHECK # undef mbsnrtowcs # if HAVE_RAW_DECL_MBSNRTOWCS _GL_WARN_ON_USE (mbsnrtowcs, "mbsnrtowcs is unportable - " "use gnulib module mbsnrtowcs for portability"); # endif #endif /* Convert a wide character to a multibyte character. */ #if @GNULIB_WCRTOMB@ # if @REPLACE_WCRTOMB@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef wcrtomb # define wcrtomb rpl_wcrtomb # endif _GL_FUNCDECL_RPL (wcrtomb, size_t, (char *s, wchar_t wc, mbstate_t *ps)); _GL_CXXALIAS_RPL (wcrtomb, size_t, (char *s, wchar_t wc, mbstate_t *ps)); # else # if !@HAVE_WCRTOMB@ _GL_FUNCDECL_SYS (wcrtomb, size_t, (char *s, wchar_t wc, mbstate_t *ps)); # endif _GL_CXXALIAS_SYS (wcrtomb, size_t, (char *s, wchar_t wc, mbstate_t *ps)); # endif _GL_CXXALIASWARN (wcrtomb); #elif defined GNULIB_POSIXCHECK # undef wcrtomb # if HAVE_RAW_DECL_WCRTOMB _GL_WARN_ON_USE (wcrtomb, "wcrtomb is unportable - " "use gnulib module wcrtomb for portability"); # endif #endif /* Convert a wide string to a string. */ #if @GNULIB_WCSRTOMBS@ # if @REPLACE_WCSRTOMBS@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef wcsrtombs # define wcsrtombs rpl_wcsrtombs # endif _GL_FUNCDECL_RPL (wcsrtombs, size_t, (char *dest, const wchar_t **srcp, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (wcsrtombs, size_t, (char *dest, const wchar_t **srcp, size_t len, mbstate_t *ps)); # else # if !@HAVE_WCSRTOMBS@ _GL_FUNCDECL_SYS (wcsrtombs, size_t, (char *dest, const wchar_t **srcp, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (wcsrtombs, size_t, (char *dest, const wchar_t **srcp, size_t len, mbstate_t *ps)); # endif _GL_CXXALIASWARN (wcsrtombs); #elif defined GNULIB_POSIXCHECK # undef wcsrtombs # if HAVE_RAW_DECL_WCSRTOMBS _GL_WARN_ON_USE (wcsrtombs, "wcsrtombs is unportable - " "use gnulib module wcsrtombs for portability"); # endif #endif /* Convert a wide string to a string. */ #if @GNULIB_WCSNRTOMBS@ # if @REPLACE_WCSNRTOMBS@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef wcsnrtombs # define wcsnrtombs rpl_wcsnrtombs # endif _GL_FUNCDECL_RPL (wcsnrtombs, size_t, (char *dest, const wchar_t **srcp, size_t srclen, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (wcsnrtombs, size_t, (char *dest, const wchar_t **srcp, size_t srclen, size_t len, mbstate_t *ps)); # else # if !@HAVE_WCSNRTOMBS@ _GL_FUNCDECL_SYS (wcsnrtombs, size_t, (char *dest, const wchar_t **srcp, size_t srclen, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (wcsnrtombs, size_t, (char *dest, const wchar_t **srcp, size_t srclen, size_t len, mbstate_t *ps)); # endif _GL_CXXALIASWARN (wcsnrtombs); #elif defined GNULIB_POSIXCHECK # undef wcsnrtombs # if HAVE_RAW_DECL_WCSNRTOMBS _GL_WARN_ON_USE (wcsnrtombs, "wcsnrtombs is unportable - " "use gnulib module wcsnrtombs for portability"); # endif #endif /* Return the number of screen columns needed for WC. */ #if @GNULIB_WCWIDTH@ # if @REPLACE_WCWIDTH@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef wcwidth # define wcwidth rpl_wcwidth # endif _GL_FUNCDECL_RPL (wcwidth, int, (wchar_t) _GL_ATTRIBUTE_PURE); _GL_CXXALIAS_RPL (wcwidth, int, (wchar_t)); # else # if !@HAVE_DECL_WCWIDTH@ /* wcwidth exists but is not declared. */ _GL_FUNCDECL_SYS (wcwidth, int, (wchar_t) _GL_ATTRIBUTE_PURE); # elif defined __KLIBC__ /* On OS/2 kLIBC, wcwidth is a macro that expands to the name of a static inline function. The implementation of wcwidth in wcwidth.c causes a "conflicting types" error. */ # undef wcwidth # endif _GL_CXXALIAS_SYS (wcwidth, int, (wchar_t)); # endif _GL_CXXALIASWARN (wcwidth); #elif defined GNULIB_POSIXCHECK # undef wcwidth # if HAVE_RAW_DECL_WCWIDTH _GL_WARN_ON_USE (wcwidth, "wcwidth is unportable - " "use gnulib module wcwidth for portability"); # endif #endif /* Search N wide characters of S for C. */ #if @GNULIB_WMEMCHR@ # if !@HAVE_WMEMCHR@ _GL_FUNCDECL_SYS (wmemchr, wchar_t *, (const wchar_t *s, wchar_t c, size_t n) _GL_ATTRIBUTE_PURE); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const wchar_t * std::wmemchr (const wchar_t *, wchar_t, size_t); wchar_t * std::wmemchr (wchar_t *, wchar_t, size_t); } */ _GL_CXXALIAS_SYS_CAST2 (wmemchr, wchar_t *, (const wchar_t *, wchar_t, size_t), const wchar_t *, (const wchar_t *, wchar_t, size_t)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (wmemchr, wchar_t *, (wchar_t *s, wchar_t c, size_t n)); _GL_CXXALIASWARN1 (wmemchr, const wchar_t *, (const wchar_t *s, wchar_t c, size_t n)); # else _GL_CXXALIASWARN (wmemchr); # endif #elif defined GNULIB_POSIXCHECK # undef wmemchr # if HAVE_RAW_DECL_WMEMCHR _GL_WARN_ON_USE (wmemchr, "wmemchr is unportable - " "use gnulib module wmemchr for portability"); # endif #endif /* Compare N wide characters of S1 and S2. */ #if @GNULIB_WMEMCMP@ # if !@HAVE_WMEMCMP@ _GL_FUNCDECL_SYS (wmemcmp, int, (const wchar_t *s1, const wchar_t *s2, size_t n) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wmemcmp, int, (const wchar_t *s1, const wchar_t *s2, size_t n)); _GL_CXXALIASWARN (wmemcmp); #elif defined GNULIB_POSIXCHECK # undef wmemcmp # if HAVE_RAW_DECL_WMEMCMP _GL_WARN_ON_USE (wmemcmp, "wmemcmp is unportable - " "use gnulib module wmemcmp for portability"); # endif #endif /* Copy N wide characters of SRC to DEST. */ #if @GNULIB_WMEMCPY@ # if !@HAVE_WMEMCPY@ _GL_FUNCDECL_SYS (wmemcpy, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); # endif _GL_CXXALIAS_SYS (wmemcpy, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); _GL_CXXALIASWARN (wmemcpy); #elif defined GNULIB_POSIXCHECK # undef wmemcpy # if HAVE_RAW_DECL_WMEMCPY _GL_WARN_ON_USE (wmemcpy, "wmemcpy is unportable - " "use gnulib module wmemcpy for portability"); # endif #endif /* Copy N wide characters of SRC to DEST, guaranteeing correct behavior for overlapping memory areas. */ #if @GNULIB_WMEMMOVE@ # if !@HAVE_WMEMMOVE@ _GL_FUNCDECL_SYS (wmemmove, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); # endif _GL_CXXALIAS_SYS (wmemmove, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); _GL_CXXALIASWARN (wmemmove); #elif defined GNULIB_POSIXCHECK # undef wmemmove # if HAVE_RAW_DECL_WMEMMOVE _GL_WARN_ON_USE (wmemmove, "wmemmove is unportable - " "use gnulib module wmemmove for portability"); # endif #endif /* Set N wide characters of S to C. */ #if @GNULIB_WMEMSET@ # if !@HAVE_WMEMSET@ _GL_FUNCDECL_SYS (wmemset, wchar_t *, (wchar_t *s, wchar_t c, size_t n)); # endif _GL_CXXALIAS_SYS (wmemset, wchar_t *, (wchar_t *s, wchar_t c, size_t n)); _GL_CXXALIASWARN (wmemset); #elif defined GNULIB_POSIXCHECK # undef wmemset # if HAVE_RAW_DECL_WMEMSET _GL_WARN_ON_USE (wmemset, "wmemset is unportable - " "use gnulib module wmemset for portability"); # endif #endif /* Return the number of wide characters in S. */ #if @GNULIB_WCSLEN@ # if !@HAVE_WCSLEN@ _GL_FUNCDECL_SYS (wcslen, size_t, (const wchar_t *s) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcslen, size_t, (const wchar_t *s)); _GL_CXXALIASWARN (wcslen); #elif defined GNULIB_POSIXCHECK # undef wcslen # if HAVE_RAW_DECL_WCSLEN _GL_WARN_ON_USE (wcslen, "wcslen is unportable - " "use gnulib module wcslen for portability"); # endif #endif /* Return the number of wide characters in S, but at most MAXLEN. */ #if @GNULIB_WCSNLEN@ # if !@HAVE_WCSNLEN@ _GL_FUNCDECL_SYS (wcsnlen, size_t, (const wchar_t *s, size_t maxlen) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcsnlen, size_t, (const wchar_t *s, size_t maxlen)); _GL_CXXALIASWARN (wcsnlen); #elif defined GNULIB_POSIXCHECK # undef wcsnlen # if HAVE_RAW_DECL_WCSNLEN _GL_WARN_ON_USE (wcsnlen, "wcsnlen is unportable - " "use gnulib module wcsnlen for portability"); # endif #endif /* Copy SRC to DEST. */ #if @GNULIB_WCSCPY@ # if !@HAVE_WCSCPY@ _GL_FUNCDECL_SYS (wcscpy, wchar_t *, (wchar_t *dest, const wchar_t *src)); # endif _GL_CXXALIAS_SYS (wcscpy, wchar_t *, (wchar_t *dest, const wchar_t *src)); _GL_CXXALIASWARN (wcscpy); #elif defined GNULIB_POSIXCHECK # undef wcscpy # if HAVE_RAW_DECL_WCSCPY _GL_WARN_ON_USE (wcscpy, "wcscpy is unportable - " "use gnulib module wcscpy for portability"); # endif #endif /* Copy SRC to DEST, returning the address of the terminating L'\0' in DEST. */ #if @GNULIB_WCPCPY@ # if !@HAVE_WCPCPY@ _GL_FUNCDECL_SYS (wcpcpy, wchar_t *, (wchar_t *dest, const wchar_t *src)); # endif _GL_CXXALIAS_SYS (wcpcpy, wchar_t *, (wchar_t *dest, const wchar_t *src)); _GL_CXXALIASWARN (wcpcpy); #elif defined GNULIB_POSIXCHECK # undef wcpcpy # if HAVE_RAW_DECL_WCPCPY _GL_WARN_ON_USE (wcpcpy, "wcpcpy is unportable - " "use gnulib module wcpcpy for portability"); # endif #endif /* Copy no more than N wide characters of SRC to DEST. */ #if @GNULIB_WCSNCPY@ # if !@HAVE_WCSNCPY@ _GL_FUNCDECL_SYS (wcsncpy, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); # endif _GL_CXXALIAS_SYS (wcsncpy, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); _GL_CXXALIASWARN (wcsncpy); #elif defined GNULIB_POSIXCHECK # undef wcsncpy # if HAVE_RAW_DECL_WCSNCPY _GL_WARN_ON_USE (wcsncpy, "wcsncpy is unportable - " "use gnulib module wcsncpy for portability"); # endif #endif /* Copy no more than N characters of SRC to DEST, returning the address of the last character written into DEST. */ #if @GNULIB_WCPNCPY@ # if !@HAVE_WCPNCPY@ _GL_FUNCDECL_SYS (wcpncpy, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); # endif _GL_CXXALIAS_SYS (wcpncpy, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); _GL_CXXALIASWARN (wcpncpy); #elif defined GNULIB_POSIXCHECK # undef wcpncpy # if HAVE_RAW_DECL_WCPNCPY _GL_WARN_ON_USE (wcpncpy, "wcpncpy is unportable - " "use gnulib module wcpncpy for portability"); # endif #endif /* Append SRC onto DEST. */ #if @GNULIB_WCSCAT@ # if !@HAVE_WCSCAT@ _GL_FUNCDECL_SYS (wcscat, wchar_t *, (wchar_t *dest, const wchar_t *src)); # endif _GL_CXXALIAS_SYS (wcscat, wchar_t *, (wchar_t *dest, const wchar_t *src)); _GL_CXXALIASWARN (wcscat); #elif defined GNULIB_POSIXCHECK # undef wcscat # if HAVE_RAW_DECL_WCSCAT _GL_WARN_ON_USE (wcscat, "wcscat is unportable - " "use gnulib module wcscat for portability"); # endif #endif /* Append no more than N wide characters of SRC onto DEST. */ #if @GNULIB_WCSNCAT@ # if !@HAVE_WCSNCAT@ _GL_FUNCDECL_SYS (wcsncat, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); # endif _GL_CXXALIAS_SYS (wcsncat, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); _GL_CXXALIASWARN (wcsncat); #elif defined GNULIB_POSIXCHECK # undef wcsncat # if HAVE_RAW_DECL_WCSNCAT _GL_WARN_ON_USE (wcsncat, "wcsncat is unportable - " "use gnulib module wcsncat for portability"); # endif #endif /* Compare S1 and S2. */ #if @GNULIB_WCSCMP@ # if !@HAVE_WCSCMP@ _GL_FUNCDECL_SYS (wcscmp, int, (const wchar_t *s1, const wchar_t *s2) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcscmp, int, (const wchar_t *s1, const wchar_t *s2)); _GL_CXXALIASWARN (wcscmp); #elif defined GNULIB_POSIXCHECK # undef wcscmp # if HAVE_RAW_DECL_WCSCMP _GL_WARN_ON_USE (wcscmp, "wcscmp is unportable - " "use gnulib module wcscmp for portability"); # endif #endif /* Compare no more than N wide characters of S1 and S2. */ #if @GNULIB_WCSNCMP@ # if !@HAVE_WCSNCMP@ _GL_FUNCDECL_SYS (wcsncmp, int, (const wchar_t *s1, const wchar_t *s2, size_t n) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcsncmp, int, (const wchar_t *s1, const wchar_t *s2, size_t n)); _GL_CXXALIASWARN (wcsncmp); #elif defined GNULIB_POSIXCHECK # undef wcsncmp # if HAVE_RAW_DECL_WCSNCMP _GL_WARN_ON_USE (wcsncmp, "wcsncmp is unportable - " "use gnulib module wcsncmp for portability"); # endif #endif /* Compare S1 and S2, ignoring case. */ #if @GNULIB_WCSCASECMP@ # if !@HAVE_WCSCASECMP@ _GL_FUNCDECL_SYS (wcscasecmp, int, (const wchar_t *s1, const wchar_t *s2) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcscasecmp, int, (const wchar_t *s1, const wchar_t *s2)); _GL_CXXALIASWARN (wcscasecmp); #elif defined GNULIB_POSIXCHECK # undef wcscasecmp # if HAVE_RAW_DECL_WCSCASECMP _GL_WARN_ON_USE (wcscasecmp, "wcscasecmp is unportable - " "use gnulib module wcscasecmp for portability"); # endif #endif /* Compare no more than N chars of S1 and S2, ignoring case. */ #if @GNULIB_WCSNCASECMP@ # if !@HAVE_WCSNCASECMP@ _GL_FUNCDECL_SYS (wcsncasecmp, int, (const wchar_t *s1, const wchar_t *s2, size_t n) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcsncasecmp, int, (const wchar_t *s1, const wchar_t *s2, size_t n)); _GL_CXXALIASWARN (wcsncasecmp); #elif defined GNULIB_POSIXCHECK # undef wcsncasecmp # if HAVE_RAW_DECL_WCSNCASECMP _GL_WARN_ON_USE (wcsncasecmp, "wcsncasecmp is unportable - " "use gnulib module wcsncasecmp for portability"); # endif #endif /* Compare S1 and S2, both interpreted as appropriate to the LC_COLLATE category of the current locale. */ #if @GNULIB_WCSCOLL@ # if !@HAVE_WCSCOLL@ _GL_FUNCDECL_SYS (wcscoll, int, (const wchar_t *s1, const wchar_t *s2)); # endif _GL_CXXALIAS_SYS (wcscoll, int, (const wchar_t *s1, const wchar_t *s2)); _GL_CXXALIASWARN (wcscoll); #elif defined GNULIB_POSIXCHECK # undef wcscoll # if HAVE_RAW_DECL_WCSCOLL _GL_WARN_ON_USE (wcscoll, "wcscoll is unportable - " "use gnulib module wcscoll for portability"); # endif #endif /* Transform S2 into array pointed to by S1 such that if wcscmp is applied to two transformed strings the result is the as applying 'wcscoll' to the original strings. */ #if @GNULIB_WCSXFRM@ # if !@HAVE_WCSXFRM@ _GL_FUNCDECL_SYS (wcsxfrm, size_t, (wchar_t *s1, const wchar_t *s2, size_t n)); # endif _GL_CXXALIAS_SYS (wcsxfrm, size_t, (wchar_t *s1, const wchar_t *s2, size_t n)); _GL_CXXALIASWARN (wcsxfrm); #elif defined GNULIB_POSIXCHECK # undef wcsxfrm # if HAVE_RAW_DECL_WCSXFRM _GL_WARN_ON_USE (wcsxfrm, "wcsxfrm is unportable - " "use gnulib module wcsxfrm for portability"); # endif #endif /* Duplicate S, returning an identical malloc'd string. */ #if @GNULIB_WCSDUP@ # if !@HAVE_WCSDUP@ _GL_FUNCDECL_SYS (wcsdup, wchar_t *, (const wchar_t *s)); # endif _GL_CXXALIAS_SYS (wcsdup, wchar_t *, (const wchar_t *s)); _GL_CXXALIASWARN (wcsdup); #elif defined GNULIB_POSIXCHECK # undef wcsdup # if HAVE_RAW_DECL_WCSDUP _GL_WARN_ON_USE (wcsdup, "wcsdup is unportable - " "use gnulib module wcsdup for portability"); # endif #endif /* Find the first occurrence of WC in WCS. */ #if @GNULIB_WCSCHR@ # if !@HAVE_WCSCHR@ _GL_FUNCDECL_SYS (wcschr, wchar_t *, (const wchar_t *wcs, wchar_t wc) _GL_ATTRIBUTE_PURE); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const wchar_t * std::wcschr (const wchar_t *, wchar_t); wchar_t * std::wcschr (wchar_t *, wchar_t); } */ _GL_CXXALIAS_SYS_CAST2 (wcschr, wchar_t *, (const wchar_t *, wchar_t), const wchar_t *, (const wchar_t *, wchar_t)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (wcschr, wchar_t *, (wchar_t *wcs, wchar_t wc)); _GL_CXXALIASWARN1 (wcschr, const wchar_t *, (const wchar_t *wcs, wchar_t wc)); # else _GL_CXXALIASWARN (wcschr); # endif #elif defined GNULIB_POSIXCHECK # undef wcschr # if HAVE_RAW_DECL_WCSCHR _GL_WARN_ON_USE (wcschr, "wcschr is unportable - " "use gnulib module wcschr for portability"); # endif #endif /* Find the last occurrence of WC in WCS. */ #if @GNULIB_WCSRCHR@ # if !@HAVE_WCSRCHR@ _GL_FUNCDECL_SYS (wcsrchr, wchar_t *, (const wchar_t *wcs, wchar_t wc) _GL_ATTRIBUTE_PURE); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const wchar_t * std::wcsrchr (const wchar_t *, wchar_t); wchar_t * std::wcsrchr (wchar_t *, wchar_t); } */ _GL_CXXALIAS_SYS_CAST2 (wcsrchr, wchar_t *, (const wchar_t *, wchar_t), const wchar_t *, (const wchar_t *, wchar_t)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (wcsrchr, wchar_t *, (wchar_t *wcs, wchar_t wc)); _GL_CXXALIASWARN1 (wcsrchr, const wchar_t *, (const wchar_t *wcs, wchar_t wc)); # else _GL_CXXALIASWARN (wcsrchr); # endif #elif defined GNULIB_POSIXCHECK # undef wcsrchr # if HAVE_RAW_DECL_WCSRCHR _GL_WARN_ON_USE (wcsrchr, "wcsrchr is unportable - " "use gnulib module wcsrchr for portability"); # endif #endif /* Return the length of the initial segmet of WCS which consists entirely of wide characters not in REJECT. */ #if @GNULIB_WCSCSPN@ # if !@HAVE_WCSCSPN@ _GL_FUNCDECL_SYS (wcscspn, size_t, (const wchar_t *wcs, const wchar_t *reject) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcscspn, size_t, (const wchar_t *wcs, const wchar_t *reject)); _GL_CXXALIASWARN (wcscspn); #elif defined GNULIB_POSIXCHECK # undef wcscspn # if HAVE_RAW_DECL_WCSCSPN _GL_WARN_ON_USE (wcscspn, "wcscspn is unportable - " "use gnulib module wcscspn for portability"); # endif #endif /* Return the length of the initial segmet of WCS which consists entirely of wide characters in ACCEPT. */ #if @GNULIB_WCSSPN@ # if !@HAVE_WCSSPN@ _GL_FUNCDECL_SYS (wcsspn, size_t, (const wchar_t *wcs, const wchar_t *accept) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcsspn, size_t, (const wchar_t *wcs, const wchar_t *accept)); _GL_CXXALIASWARN (wcsspn); #elif defined GNULIB_POSIXCHECK # undef wcsspn # if HAVE_RAW_DECL_WCSSPN _GL_WARN_ON_USE (wcsspn, "wcsspn is unportable - " "use gnulib module wcsspn for portability"); # endif #endif /* Find the first occurrence in WCS of any character in ACCEPT. */ #if @GNULIB_WCSPBRK@ # if !@HAVE_WCSPBRK@ _GL_FUNCDECL_SYS (wcspbrk, wchar_t *, (const wchar_t *wcs, const wchar_t *accept) _GL_ATTRIBUTE_PURE); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const wchar_t * std::wcspbrk (const wchar_t *, const wchar_t *); wchar_t * std::wcspbrk (wchar_t *, const wchar_t *); } */ _GL_CXXALIAS_SYS_CAST2 (wcspbrk, wchar_t *, (const wchar_t *, const wchar_t *), const wchar_t *, (const wchar_t *, const wchar_t *)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (wcspbrk, wchar_t *, (wchar_t *wcs, const wchar_t *accept)); _GL_CXXALIASWARN1 (wcspbrk, const wchar_t *, (const wchar_t *wcs, const wchar_t *accept)); # else _GL_CXXALIASWARN (wcspbrk); # endif #elif defined GNULIB_POSIXCHECK # undef wcspbrk # if HAVE_RAW_DECL_WCSPBRK _GL_WARN_ON_USE (wcspbrk, "wcspbrk is unportable - " "use gnulib module wcspbrk for portability"); # endif #endif /* Find the first occurrence of NEEDLE in HAYSTACK. */ #if @GNULIB_WCSSTR@ # if !@HAVE_WCSSTR@ _GL_FUNCDECL_SYS (wcsstr, wchar_t *, (const wchar_t *haystack, const wchar_t *needle) _GL_ATTRIBUTE_PURE); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const wchar_t * std::wcsstr (const wchar_t *, const wchar_t *); wchar_t * std::wcsstr (wchar_t *, const wchar_t *); } */ _GL_CXXALIAS_SYS_CAST2 (wcsstr, wchar_t *, (const wchar_t *, const wchar_t *), const wchar_t *, (const wchar_t *, const wchar_t *)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (wcsstr, wchar_t *, (wchar_t *haystack, const wchar_t *needle)); _GL_CXXALIASWARN1 (wcsstr, const wchar_t *, (const wchar_t *haystack, const wchar_t *needle)); # else _GL_CXXALIASWARN (wcsstr); # endif #elif defined GNULIB_POSIXCHECK # undef wcsstr # if HAVE_RAW_DECL_WCSSTR _GL_WARN_ON_USE (wcsstr, "wcsstr is unportable - " "use gnulib module wcsstr for portability"); # endif #endif /* Divide WCS into tokens separated by characters in DELIM. */ #if @GNULIB_WCSTOK@ # if !@HAVE_WCSTOK@ _GL_FUNCDECL_SYS (wcstok, wchar_t *, (wchar_t *wcs, const wchar_t *delim, wchar_t **ptr)); # endif _GL_CXXALIAS_SYS (wcstok, wchar_t *, (wchar_t *wcs, const wchar_t *delim, wchar_t **ptr)); _GL_CXXALIASWARN (wcstok); #elif defined GNULIB_POSIXCHECK # undef wcstok # if HAVE_RAW_DECL_WCSTOK _GL_WARN_ON_USE (wcstok, "wcstok is unportable - " "use gnulib module wcstok for portability"); # endif #endif /* Determine number of column positions required for first N wide characters (or fewer if S ends before this) in S. */ #if @GNULIB_WCSWIDTH@ # if @REPLACE_WCSWIDTH@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef wcswidth # define wcswidth rpl_wcswidth # endif _GL_FUNCDECL_RPL (wcswidth, int, (const wchar_t *s, size_t n) _GL_ATTRIBUTE_PURE); _GL_CXXALIAS_RPL (wcswidth, int, (const wchar_t *s, size_t n)); # else # if !@HAVE_WCSWIDTH@ _GL_FUNCDECL_SYS (wcswidth, int, (const wchar_t *s, size_t n) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcswidth, int, (const wchar_t *s, size_t n)); # endif _GL_CXXALIASWARN (wcswidth); #elif defined GNULIB_POSIXCHECK # undef wcswidth # if HAVE_RAW_DECL_WCSWIDTH _GL_WARN_ON_USE (wcswidth, "wcswidth is unportable - " "use gnulib module wcswidth for portability"); # endif #endif #endif /* _@GUARD_PREFIX@_WCHAR_H */ #endif /* _@GUARD_PREFIX@_WCHAR_H */ #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/verify.h0000644000175000017500000002541213004436754016060 00000000000000/* Compile-time assert-like macros. Copyright (C) 2005-2006, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paul Eggert, Bruno Haible, and Jim Meyering. */ #ifndef _GL_VERIFY_H #define _GL_VERIFY_H /* Define _GL_HAVE__STATIC_ASSERT to 1 if _Static_assert works as per C11. This is supported by GCC 4.6.0 and later, in C mode, and its use here generates easier-to-read diagnostics when verify (R) fails. Define _GL_HAVE_STATIC_ASSERT to 1 if static_assert works as per C++11. This will likely be supported by future GCC versions, in C++ mode. Use this only with GCC. If we were willing to slow 'configure' down we could also use it with other compilers, but since this affects only the quality of diagnostics, why bother? */ #if (4 < __GNUC__ + (6 <= __GNUC_MINOR__) \ && (201112L <= __STDC_VERSION__ || !defined __STRICT_ANSI__) \ && !defined __cplusplus) # define _GL_HAVE__STATIC_ASSERT 1 #endif /* The condition (99 < __GNUC__) is temporary, until we know about the first G++ release that supports static_assert. */ #if (99 < __GNUC__) && defined __cplusplus # define _GL_HAVE_STATIC_ASSERT 1 #endif /* FreeBSD 9.1 , included by and lots of other system headers, defines a conflicting _Static_assert that is no better than ours; override it. */ #ifndef _GL_HAVE_STATIC_ASSERT # include # undef _Static_assert #endif /* Each of these macros verifies that its argument R is nonzero. To be portable, R should be an integer constant expression. Unlike assert (R), there is no run-time overhead. If _Static_assert works, verify (R) uses it directly. Similarly, _GL_VERIFY_TRUE works by packaging a _Static_assert inside a struct that is an operand of sizeof. The code below uses several ideas for C++ compilers, and for C compilers that do not support _Static_assert: * The first step is ((R) ? 1 : -1). Given an expression R, of integral or boolean or floating-point type, this yields an expression of integral type, whose value is later verified to be constant and nonnegative. * Next this expression W is wrapped in a type struct _gl_verify_type { unsigned int _gl_verify_error_if_negative: W; }. If W is negative, this yields a compile-time error. No compiler can deal with a bit-field of negative size. One might think that an array size check would have the same effect, that is, that the type struct { unsigned int dummy[W]; } would work as well. However, inside a function, some compilers (such as C++ compilers and GNU C) allow local parameters and variables inside array size expressions. With these compilers, an array size check would not properly diagnose this misuse of the verify macro: void function (int n) { verify (n < 0); } * For the verify macro, the struct _gl_verify_type will need to somehow be embedded into a declaration. To be portable, this declaration must declare an object, a constant, a function, or a typedef name. If the declared entity uses the type directly, such as in struct dummy {...}; typedef struct {...} dummy; extern struct {...} *dummy; extern void dummy (struct {...} *); extern struct {...} *dummy (void); two uses of the verify macro would yield colliding declarations if the entity names are not disambiguated. A workaround is to attach the current line number to the entity name: #define _GL_CONCAT0(x, y) x##y #define _GL_CONCAT(x, y) _GL_CONCAT0 (x, y) extern struct {...} * _GL_CONCAT (dummy, __LINE__); But this has the problem that two invocations of verify from within the same macro would collide, since the __LINE__ value would be the same for both invocations. (The GCC __COUNTER__ macro solves this problem, but is not portable.) A solution is to use the sizeof operator. It yields a number, getting rid of the identity of the type. Declarations like extern int dummy [sizeof (struct {...})]; extern void dummy (int [sizeof (struct {...})]); extern int (*dummy (void)) [sizeof (struct {...})]; can be repeated. * Should the implementation use a named struct or an unnamed struct? Which of the following alternatives can be used? extern int dummy [sizeof (struct {...})]; extern int dummy [sizeof (struct _gl_verify_type {...})]; extern void dummy (int [sizeof (struct {...})]); extern void dummy (int [sizeof (struct _gl_verify_type {...})]); extern int (*dummy (void)) [sizeof (struct {...})]; extern int (*dummy (void)) [sizeof (struct _gl_verify_type {...})]; In the second and sixth case, the struct type is exported to the outer scope; two such declarations therefore collide. GCC warns about the first, third, and fourth cases. So the only remaining possibility is the fifth case: extern int (*dummy (void)) [sizeof (struct {...})]; * GCC warns about duplicate declarations of the dummy function if -Wredundant-decls is used. GCC 4.3 and later have a builtin __COUNTER__ macro that can let us generate unique identifiers for each dummy function, to suppress this warning. * This implementation exploits the fact that older versions of GCC, which do not support _Static_assert, also do not warn about the last declaration mentioned above. * GCC warns if -Wnested-externs is enabled and verify() is used within a function body; but inside a function, you can always arrange to use verify_expr() instead. * In C++, any struct definition inside sizeof is invalid. Use a template type to work around the problem. */ /* Concatenate two preprocessor tokens. */ #define _GL_CONCAT(x, y) _GL_CONCAT0 (x, y) #define _GL_CONCAT0(x, y) x##y /* _GL_COUNTER is an integer, preferably one that changes each time we use it. Use __COUNTER__ if it works, falling back on __LINE__ otherwise. __LINE__ isn't perfect, but it's better than a constant. */ #if defined __COUNTER__ && __COUNTER__ != __COUNTER__ # define _GL_COUNTER __COUNTER__ #else # define _GL_COUNTER __LINE__ #endif /* Generate a symbol with the given prefix, making it unique if possible. */ #define _GL_GENSYM(prefix) _GL_CONCAT (prefix, _GL_COUNTER) /* Verify requirement R at compile-time, as an integer constant expression that returns 1. If R is false, fail at compile-time, preferably with a diagnostic that includes the string-literal DIAGNOSTIC. */ #define _GL_VERIFY_TRUE(R, DIAGNOSTIC) \ (!!sizeof (_GL_VERIFY_TYPE (R, DIAGNOSTIC))) #ifdef __cplusplus # if !GNULIB_defined_struct__gl_verify_type template struct _gl_verify_type { unsigned int _gl_verify_error_if_negative: w; }; # define GNULIB_defined_struct__gl_verify_type 1 # endif # define _GL_VERIFY_TYPE(R, DIAGNOSTIC) \ _gl_verify_type<(R) ? 1 : -1> #elif defined _GL_HAVE__STATIC_ASSERT # define _GL_VERIFY_TYPE(R, DIAGNOSTIC) \ struct { \ _Static_assert (R, DIAGNOSTIC); \ int _gl_dummy; \ } #else # define _GL_VERIFY_TYPE(R, DIAGNOSTIC) \ struct { unsigned int _gl_verify_error_if_negative: (R) ? 1 : -1; } #endif /* Verify requirement R at compile-time, as a declaration without a trailing ';'. If R is false, fail at compile-time, preferably with a diagnostic that includes the string-literal DIAGNOSTIC. Unfortunately, unlike C11, this implementation must appear as an ordinary declaration, and cannot appear inside struct { ... }. */ #ifdef _GL_HAVE__STATIC_ASSERT # define _GL_VERIFY _Static_assert #else # define _GL_VERIFY(R, DIAGNOSTIC) \ extern int (*_GL_GENSYM (_gl_verify_function) (void)) \ [_GL_VERIFY_TRUE (R, DIAGNOSTIC)] #endif /* _GL_STATIC_ASSERT_H is defined if this code is copied into assert.h. */ #ifdef _GL_STATIC_ASSERT_H # if !defined _GL_HAVE__STATIC_ASSERT && !defined _Static_assert # define _Static_assert(R, DIAGNOSTIC) _GL_VERIFY (R, DIAGNOSTIC) # endif # if !defined _GL_HAVE_STATIC_ASSERT && !defined static_assert # define static_assert _Static_assert /* C11 requires this #define. */ # endif #endif /* @assert.h omit start@ */ /* Each of these macros verifies that its argument R is nonzero. To be portable, R should be an integer constant expression. Unlike assert (R), there is no run-time overhead. There are two macros, since no single macro can be used in all contexts in C. verify_true (R) is for scalar contexts, including integer constant expression contexts. verify (R) is for declaration contexts, e.g., the top level. */ /* Verify requirement R at compile-time, as an integer constant expression. Return 1. This is equivalent to verify_expr (R, 1). verify_true is obsolescent; please use verify_expr instead. */ #define verify_true(R) _GL_VERIFY_TRUE (R, "verify_true (" #R ")") /* Verify requirement R at compile-time. Return the value of the expression E. */ #define verify_expr(R, E) \ (_GL_VERIFY_TRUE (R, "verify_expr (" #R ", " #E ")") ? (E) : (E)) /* Verify requirement R at compile-time, as a declaration without a trailing ';'. */ #define verify(R) _GL_VERIFY (R, "verify (" #R ")") #ifndef __has_builtin # define __has_builtin(x) 0 #endif /* Assume that R always holds. This lets the compiler optimize accordingly. R should not have side-effects; it may or may not be evaluated. Behavior is undefined if R is false. */ #if (__has_builtin (__builtin_unreachable) \ || 4 < __GNUC__ + (5 <= __GNUC_MINOR__)) # define assume(R) ((R) ? (void) 0 : __builtin_unreachable ()) #elif 1200 <= _MSC_VER # define assume(R) __assume (R) #elif ((defined GCC_LINT || defined lint) \ && (__has_builtin (__builtin_trap) \ || 3 < __GNUC__ + (3 < __GNUC_MINOR__ + (4 <= __GNUC_PATCHLEVEL__)))) /* Doing it this way helps various packages when configured with --enable-gcc-warnings, which compiles with -Dlint. It's nicer when 'assume' silences warnings even with older GCCs. */ # define assume(R) ((R) ? (void) 0 : __builtin_trap ()) #else # define assume(R) ((void) (0 && (R))) #endif /* @assert.h omit end@ */ #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/vasnprintf.h0000644000175000017500000000560013004436754016743 00000000000000/* vsprintf with automatic memory allocation. Copyright (C) 2002-2004, 2007-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _VASNPRINTF_H #define _VASNPRINTF_H /* Get va_list. */ #include /* Get size_t. */ #include /* The __attribute__ feature is available in gcc versions 2.5 and later. The __-protected variants of the attributes 'format' and 'printf' are accepted by gcc versions 2.6.4 (effectively 2.7) and later. We enable _GL_ATTRIBUTE_FORMAT only if these are supported too, because gnulib and libintl do '#define printf __printf__' when they override the 'printf' function. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 7) # define _GL_ATTRIBUTE_FORMAT(spec) __attribute__ ((__format__ spec)) #else # define _GL_ATTRIBUTE_FORMAT(spec) /* empty */ #endif #ifdef __cplusplus extern "C" { #endif /* Write formatted output to a string dynamically allocated with malloc(). You can pass a preallocated buffer for the result in RESULTBUF and its size in *LENGTHP; otherwise you pass RESULTBUF = NULL. If successful, return the address of the string (this may be = RESULTBUF if no dynamic memory allocation was necessary) and set *LENGTHP to the number of resulting bytes, excluding the trailing NUL. Upon error, set errno and return NULL. When dynamic memory allocation occurs, the preallocated buffer is left alone (with possibly modified contents). This makes it possible to use a statically allocated or stack-allocated buffer, like this: char buf[100]; size_t len = sizeof (buf); char *output = vasnprintf (buf, &len, format, args); if (output == NULL) ... error handling ...; else { ... use the output string ...; if (output != buf) free (output); } */ #if REPLACE_VASNPRINTF # define asnprintf rpl_asnprintf # define vasnprintf rpl_vasnprintf #endif extern char * asnprintf (char *resultbuf, size_t *lengthp, const char *format, ...) _GL_ATTRIBUTE_FORMAT ((__printf__, 3, 4)); extern char * vasnprintf (char *resultbuf, size_t *lengthp, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT ((__printf__, 3, 0)); #ifdef __cplusplus } #endif #endif /* _VASNPRINTF_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/printf-parse.h0000644000175000017500000001216313004436754017165 00000000000000/* Parse printf format string. Copyright (C) 1999, 2002-2003, 2005, 2007, 2010-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _PRINTF_PARSE_H #define _PRINTF_PARSE_H /* This file can be parametrized with the following macros: ENABLE_UNISTDIO Set to 1 to enable the unistdio extensions. STATIC Set to 'static' to declare the function static. */ #if HAVE_FEATURES_H # include /* for __GLIBC__, __UCLIBC__ */ #endif #include "printf-args.h" /* Flags */ #define FLAG_GROUP 1 /* ' flag */ #define FLAG_LEFT 2 /* - flag */ #define FLAG_SHOWSIGN 4 /* + flag */ #define FLAG_SPACE 8 /* space flag */ #define FLAG_ALT 16 /* # flag */ #define FLAG_ZERO 32 #if __GLIBC__ >= 2 && !defined __UCLIBC__ # define FLAG_LOCALIZED 64 /* I flag, uses localized digits */ #endif /* arg_index value indicating that no argument is consumed. */ #define ARG_NONE (~(size_t)0) /* xxx_directive: A parsed directive. xxx_directives: A parsed format string. */ /* Number of directly allocated directives (no malloc() needed). */ #define N_DIRECT_ALLOC_DIRECTIVES 7 /* A parsed directive. */ typedef struct { const char* dir_start; const char* dir_end; int flags; const char* width_start; const char* width_end; size_t width_arg_index; const char* precision_start; const char* precision_end; size_t precision_arg_index; char conversion; /* d i o u x X f F e E g G a A c s p n U % but not C S */ size_t arg_index; } char_directive; /* A parsed format string. */ typedef struct { size_t count; char_directive *dir; size_t max_width_length; size_t max_precision_length; char_directive direct_alloc_dir[N_DIRECT_ALLOC_DIRECTIVES]; } char_directives; #if ENABLE_UNISTDIO /* A parsed directive. */ typedef struct { const uint8_t* dir_start; const uint8_t* dir_end; int flags; const uint8_t* width_start; const uint8_t* width_end; size_t width_arg_index; const uint8_t* precision_start; const uint8_t* precision_end; size_t precision_arg_index; uint8_t conversion; /* d i o u x X f F e E g G a A c s p n U % but not C S */ size_t arg_index; } u8_directive; /* A parsed format string. */ typedef struct { size_t count; u8_directive *dir; size_t max_width_length; size_t max_precision_length; u8_directive direct_alloc_dir[N_DIRECT_ALLOC_DIRECTIVES]; } u8_directives; /* A parsed directive. */ typedef struct { const uint16_t* dir_start; const uint16_t* dir_end; int flags; const uint16_t* width_start; const uint16_t* width_end; size_t width_arg_index; const uint16_t* precision_start; const uint16_t* precision_end; size_t precision_arg_index; uint16_t conversion; /* d i o u x X f F e E g G a A c s p n U % but not C S */ size_t arg_index; } u16_directive; /* A parsed format string. */ typedef struct { size_t count; u16_directive *dir; size_t max_width_length; size_t max_precision_length; u16_directive direct_alloc_dir[N_DIRECT_ALLOC_DIRECTIVES]; } u16_directives; /* A parsed directive. */ typedef struct { const uint32_t* dir_start; const uint32_t* dir_end; int flags; const uint32_t* width_start; const uint32_t* width_end; size_t width_arg_index; const uint32_t* precision_start; const uint32_t* precision_end; size_t precision_arg_index; uint32_t conversion; /* d i o u x X f F e E g G a A c s p n U % but not C S */ size_t arg_index; } u32_directive; /* A parsed format string. */ typedef struct { size_t count; u32_directive *dir; size_t max_width_length; size_t max_precision_length; u32_directive direct_alloc_dir[N_DIRECT_ALLOC_DIRECTIVES]; } u32_directives; #endif /* Parses the format string. Fills in the number N of directives, and fills in directives[0], ..., directives[N-1], and sets directives[N].dir_start to the end of the format string. Also fills in the arg_type fields of the arguments and the needed count of arguments. */ #if ENABLE_UNISTDIO extern int ulc_printf_parse (const char *format, char_directives *d, arguments *a); extern int u8_printf_parse (const uint8_t *format, u8_directives *d, arguments *a); extern int u16_printf_parse (const uint16_t *format, u16_directives *d, arguments *a); extern int u32_printf_parse (const uint32_t *format, u32_directives *d, arguments *a); #else # ifdef STATIC STATIC # else extern # endif int printf_parse (const char *format, char_directives *d, arguments *a); #endif #endif /* _PRINTF_PARSE_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/printf-args.h0000644000175000017500000000753313004436754017014 00000000000000/* Decomposed printf argument list. Copyright (C) 1999, 2002-2003, 2006-2007, 2011-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _PRINTF_ARGS_H #define _PRINTF_ARGS_H /* This file can be parametrized with the following macros: ENABLE_UNISTDIO Set to 1 to enable the unistdio extensions. PRINTF_FETCHARGS Name of the function to be declared. STATIC Set to 'static' to declare the function static. */ /* Default parameters. */ #ifndef PRINTF_FETCHARGS # define PRINTF_FETCHARGS printf_fetchargs #endif /* Get size_t. */ #include /* Get wchar_t. */ #if HAVE_WCHAR_T # include #endif /* Get wint_t. */ #if HAVE_WINT_T # include #endif /* Get va_list. */ #include /* Argument types */ typedef enum { TYPE_NONE, TYPE_SCHAR, TYPE_UCHAR, TYPE_SHORT, TYPE_USHORT, TYPE_INT, TYPE_UINT, TYPE_LONGINT, TYPE_ULONGINT, #if HAVE_LONG_LONG_INT TYPE_LONGLONGINT, TYPE_ULONGLONGINT, #endif TYPE_DOUBLE, TYPE_LONGDOUBLE, TYPE_CHAR, #if HAVE_WINT_T TYPE_WIDE_CHAR, #endif TYPE_STRING, #if HAVE_WCHAR_T TYPE_WIDE_STRING, #endif TYPE_POINTER, TYPE_COUNT_SCHAR_POINTER, TYPE_COUNT_SHORT_POINTER, TYPE_COUNT_INT_POINTER, TYPE_COUNT_LONGINT_POINTER #if HAVE_LONG_LONG_INT , TYPE_COUNT_LONGLONGINT_POINTER #endif #if ENABLE_UNISTDIO /* The unistdio extensions. */ , TYPE_U8_STRING , TYPE_U16_STRING , TYPE_U32_STRING #endif } arg_type; /* Polymorphic argument */ typedef struct { arg_type type; union { signed char a_schar; unsigned char a_uchar; short a_short; unsigned short a_ushort; int a_int; unsigned int a_uint; long int a_longint; unsigned long int a_ulongint; #if HAVE_LONG_LONG_INT long long int a_longlongint; unsigned long long int a_ulonglongint; #endif float a_float; double a_double; long double a_longdouble; int a_char; #if HAVE_WINT_T wint_t a_wide_char; #endif const char* a_string; #if HAVE_WCHAR_T const wchar_t* a_wide_string; #endif void* a_pointer; signed char * a_count_schar_pointer; short * a_count_short_pointer; int * a_count_int_pointer; long int * a_count_longint_pointer; #if HAVE_LONG_LONG_INT long long int * a_count_longlongint_pointer; #endif #if ENABLE_UNISTDIO /* The unistdio extensions. */ const uint8_t * a_u8_string; const uint16_t * a_u16_string; const uint32_t * a_u32_string; #endif } a; } argument; /* Number of directly allocated arguments (no malloc() needed). */ #define N_DIRECT_ALLOC_ARGUMENTS 7 typedef struct { size_t count; argument *arg; argument direct_alloc_arg[N_DIRECT_ALLOC_ARGUMENTS]; } arguments; /* Fetch the arguments, putting them into a. */ #ifdef STATIC STATIC #else extern #endif int PRINTF_FETCHARGS (va_list args, arguments *a); #endif /* _PRINTF_ARGS_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/float+.h0000644000175000017500000001274513004436754015741 00000000000000/* Supplemental information about the floating-point formats. Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2007. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _FLOATPLUS_H #define _FLOATPLUS_H #include #include /* Number of bits in the mantissa of a floating-point number, including the "hidden bit". */ #if FLT_RADIX == 2 # define FLT_MANT_BIT FLT_MANT_DIG # define DBL_MANT_BIT DBL_MANT_DIG # define LDBL_MANT_BIT LDBL_MANT_DIG #elif FLT_RADIX == 4 # define FLT_MANT_BIT (FLT_MANT_DIG * 2) # define DBL_MANT_BIT (DBL_MANT_DIG * 2) # define LDBL_MANT_BIT (LDBL_MANT_DIG * 2) #elif FLT_RADIX == 16 # define FLT_MANT_BIT (FLT_MANT_DIG * 4) # define DBL_MANT_BIT (DBL_MANT_DIG * 4) # define LDBL_MANT_BIT (LDBL_MANT_DIG * 4) #endif /* Bit mask that can be used to mask the exponent, as an unsigned number. */ #define FLT_EXP_MASK ((FLT_MAX_EXP - FLT_MIN_EXP) | 7) #define DBL_EXP_MASK ((DBL_MAX_EXP - DBL_MIN_EXP) | 7) #define LDBL_EXP_MASK ((LDBL_MAX_EXP - LDBL_MIN_EXP) | 7) /* Number of bits used for the exponent of a floating-point number, including the exponent's sign. */ #define FLT_EXP_BIT \ (FLT_EXP_MASK < 0x100 ? 8 : \ FLT_EXP_MASK < 0x200 ? 9 : \ FLT_EXP_MASK < 0x400 ? 10 : \ FLT_EXP_MASK < 0x800 ? 11 : \ FLT_EXP_MASK < 0x1000 ? 12 : \ FLT_EXP_MASK < 0x2000 ? 13 : \ FLT_EXP_MASK < 0x4000 ? 14 : \ FLT_EXP_MASK < 0x8000 ? 15 : \ FLT_EXP_MASK < 0x10000 ? 16 : \ FLT_EXP_MASK < 0x20000 ? 17 : \ FLT_EXP_MASK < 0x40000 ? 18 : \ FLT_EXP_MASK < 0x80000 ? 19 : \ FLT_EXP_MASK < 0x100000 ? 20 : \ FLT_EXP_MASK < 0x200000 ? 21 : \ FLT_EXP_MASK < 0x400000 ? 22 : \ FLT_EXP_MASK < 0x800000 ? 23 : \ FLT_EXP_MASK < 0x1000000 ? 24 : \ FLT_EXP_MASK < 0x2000000 ? 25 : \ FLT_EXP_MASK < 0x4000000 ? 26 : \ FLT_EXP_MASK < 0x8000000 ? 27 : \ FLT_EXP_MASK < 0x10000000 ? 28 : \ FLT_EXP_MASK < 0x20000000 ? 29 : \ FLT_EXP_MASK < 0x40000000 ? 30 : \ FLT_EXP_MASK <= 0x7fffffff ? 31 : \ 32) #define DBL_EXP_BIT \ (DBL_EXP_MASK < 0x100 ? 8 : \ DBL_EXP_MASK < 0x200 ? 9 : \ DBL_EXP_MASK < 0x400 ? 10 : \ DBL_EXP_MASK < 0x800 ? 11 : \ DBL_EXP_MASK < 0x1000 ? 12 : \ DBL_EXP_MASK < 0x2000 ? 13 : \ DBL_EXP_MASK < 0x4000 ? 14 : \ DBL_EXP_MASK < 0x8000 ? 15 : \ DBL_EXP_MASK < 0x10000 ? 16 : \ DBL_EXP_MASK < 0x20000 ? 17 : \ DBL_EXP_MASK < 0x40000 ? 18 : \ DBL_EXP_MASK < 0x80000 ? 19 : \ DBL_EXP_MASK < 0x100000 ? 20 : \ DBL_EXP_MASK < 0x200000 ? 21 : \ DBL_EXP_MASK < 0x400000 ? 22 : \ DBL_EXP_MASK < 0x800000 ? 23 : \ DBL_EXP_MASK < 0x1000000 ? 24 : \ DBL_EXP_MASK < 0x2000000 ? 25 : \ DBL_EXP_MASK < 0x4000000 ? 26 : \ DBL_EXP_MASK < 0x8000000 ? 27 : \ DBL_EXP_MASK < 0x10000000 ? 28 : \ DBL_EXP_MASK < 0x20000000 ? 29 : \ DBL_EXP_MASK < 0x40000000 ? 30 : \ DBL_EXP_MASK <= 0x7fffffff ? 31 : \ 32) #define LDBL_EXP_BIT \ (LDBL_EXP_MASK < 0x100 ? 8 : \ LDBL_EXP_MASK < 0x200 ? 9 : \ LDBL_EXP_MASK < 0x400 ? 10 : \ LDBL_EXP_MASK < 0x800 ? 11 : \ LDBL_EXP_MASK < 0x1000 ? 12 : \ LDBL_EXP_MASK < 0x2000 ? 13 : \ LDBL_EXP_MASK < 0x4000 ? 14 : \ LDBL_EXP_MASK < 0x8000 ? 15 : \ LDBL_EXP_MASK < 0x10000 ? 16 : \ LDBL_EXP_MASK < 0x20000 ? 17 : \ LDBL_EXP_MASK < 0x40000 ? 18 : \ LDBL_EXP_MASK < 0x80000 ? 19 : \ LDBL_EXP_MASK < 0x100000 ? 20 : \ LDBL_EXP_MASK < 0x200000 ? 21 : \ LDBL_EXP_MASK < 0x400000 ? 22 : \ LDBL_EXP_MASK < 0x800000 ? 23 : \ LDBL_EXP_MASK < 0x1000000 ? 24 : \ LDBL_EXP_MASK < 0x2000000 ? 25 : \ LDBL_EXP_MASK < 0x4000000 ? 26 : \ LDBL_EXP_MASK < 0x8000000 ? 27 : \ LDBL_EXP_MASK < 0x10000000 ? 28 : \ LDBL_EXP_MASK < 0x20000000 ? 29 : \ LDBL_EXP_MASK < 0x40000000 ? 30 : \ LDBL_EXP_MASK <= 0x7fffffff ? 31 : \ 32) /* Number of bits used for a floating-point number: the mantissa (not counting the "hidden bit", since it may or may not be explicit), the exponent, and the sign. */ #define FLT_TOTAL_BIT ((FLT_MANT_BIT - 1) + FLT_EXP_BIT + 1) #define DBL_TOTAL_BIT ((DBL_MANT_BIT - 1) + DBL_EXP_BIT + 1) #define LDBL_TOTAL_BIT ((LDBL_MANT_BIT - 1) + LDBL_EXP_BIT + 1) /* Number of bytes used for a floating-point number. This can be smaller than the 'sizeof'. For example, on i386 systems, 'long double' most often have LDBL_MANT_BIT = 64, LDBL_EXP_BIT = 16, hence LDBL_TOTAL_BIT = 80 bits, i.e. 10 bytes of consecutive memory, but sizeof (long double) = 12 or = 16. */ #define SIZEOF_FLT ((FLT_TOTAL_BIT + CHAR_BIT - 1) / CHAR_BIT) #define SIZEOF_DBL ((DBL_TOTAL_BIT + CHAR_BIT - 1) / CHAR_BIT) #define SIZEOF_LDBL ((LDBL_TOTAL_BIT + CHAR_BIT - 1) / CHAR_BIT) /* Verify that SIZEOF_FLT <= sizeof (float) etc. */ typedef int verify_sizeof_flt[SIZEOF_FLT <= sizeof (float) ? 1 : -1]; typedef int verify_sizeof_dbl[SIZEOF_DBL <= sizeof (double) ? 1 : - 1]; typedef int verify_sizeof_ldbl[SIZEOF_LDBL <= sizeof (long double) ? 1 : - 1]; #endif /* _FLOATPLUS_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/unistd.in.h0000644000175000017500000015100013004436754016460 00000000000000/* Substitute for and wrapper around . Copyright (C) 2003-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _@GUARD_PREFIX@_UNISTD_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #ifdef _GL_INCLUDING_UNISTD_H /* Special invocation convention: - On Mac OS X 10.3.9 we have a sequence of nested includes -> -> -> In this situation, the functions are not yet declared, therefore we cannot provide the C++ aliases. */ #@INCLUDE_NEXT@ @NEXT_UNISTD_H@ #else /* Normal invocation convention. */ /* The include_next requires a split double-inclusion guard. */ #if @HAVE_UNISTD_H@ # define _GL_INCLUDING_UNISTD_H # @INCLUDE_NEXT@ @NEXT_UNISTD_H@ # undef _GL_INCLUDING_UNISTD_H #endif /* Get all possible declarations of gethostname(). */ #if @GNULIB_GETHOSTNAME@ && @UNISTD_H_HAVE_WINSOCK2_H@ \ && !defined _GL_INCLUDING_WINSOCK2_H # define _GL_INCLUDING_WINSOCK2_H # include # undef _GL_INCLUDING_WINSOCK2_H #endif #if !defined _@GUARD_PREFIX@_UNISTD_H && !defined _GL_INCLUDING_WINSOCK2_H #define _@GUARD_PREFIX@_UNISTD_H /* NetBSD 5.0 mis-defines NULL. Also get size_t. */ #include /* mingw doesn't define the SEEK_* or *_FILENO macros in . */ /* Cygwin 1.7.1 declares symlinkat in , not in . */ /* But avoid namespace pollution on glibc systems. */ #if (!(defined SEEK_CUR && defined SEEK_END && defined SEEK_SET) \ || ((@GNULIB_SYMLINKAT@ || defined GNULIB_POSIXCHECK) \ && defined __CYGWIN__)) \ && ! defined __GLIBC__ # include #endif /* Cygwin 1.7.1 declares unlinkat in , not in . */ /* But avoid namespace pollution on glibc systems. */ #if (@GNULIB_UNLINKAT@ || defined GNULIB_POSIXCHECK) && defined __CYGWIN__ \ && ! defined __GLIBC__ # include #endif /* mingw fails to declare _exit in . */ /* mingw, MSVC, BeOS, Haiku declare environ in , not in . */ /* Solaris declares getcwd not only in but also in . */ /* OSF Tru64 Unix cannot see gnulib rpl_strtod when system is included here. */ /* But avoid namespace pollution on glibc systems. */ #if !defined __GLIBC__ && !defined __osf__ # define __need_system_stdlib_h # include # undef __need_system_stdlib_h #endif /* Native Windows platforms declare chdir, getcwd, rmdir in and/or , not in . They also declare access(), chmod(), close(), dup(), dup2(), isatty(), lseek(), read(), unlink(), write() in . */ #if ((@GNULIB_CHDIR@ || @GNULIB_GETCWD@ || @GNULIB_RMDIR@ \ || defined GNULIB_POSIXCHECK) \ && ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__)) # include /* mingw32, mingw64 */ # include /* mingw64, MSVC 9 */ #elif (@GNULIB_CLOSE@ || @GNULIB_DUP@ || @GNULIB_DUP2@ || @GNULIB_ISATTY@ \ || @GNULIB_LSEEK@ || @GNULIB_READ@ || @GNULIB_UNLINK@ || @GNULIB_WRITE@ \ || defined GNULIB_POSIXCHECK) \ && ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) # include #endif /* AIX and OSF/1 5.1 declare getdomainname in , not in . NonStop Kernel declares gethostname in , not in . */ /* But avoid namespace pollution on glibc systems. */ #if ((@GNULIB_GETDOMAINNAME@ && (defined _AIX || defined __osf__)) \ || (@GNULIB_GETHOSTNAME@ && defined __TANDEM)) \ && !defined __GLIBC__ # include #endif /* MSVC defines off_t in . May also define off_t to a 64-bit type on native Windows. */ #if !@HAVE_UNISTD_H@ || @WINDOWS_64_BIT_OFF_T@ /* Get off_t. */ # include #endif #if (@GNULIB_READ@ || @GNULIB_WRITE@ \ || @GNULIB_READLINK@ || @GNULIB_READLINKAT@ \ || @GNULIB_PREAD@ || @GNULIB_PWRITE@ || defined GNULIB_POSIXCHECK) /* Get ssize_t. */ # include #endif /* Get getopt(), optarg, optind, opterr, optopt. But avoid namespace pollution on glibc systems. */ #if @GNULIB_UNISTD_H_GETOPT@ && !defined __GLIBC__ && !defined _GL_SYSTEM_GETOPT # define __need_getopt # include #endif #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef _GL_UNISTD_INLINE # define _GL_UNISTD_INLINE _GL_INLINE #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Hide some function declarations from . */ #if @GNULIB_GETHOSTNAME@ && @UNISTD_H_HAVE_WINSOCK2_H@ # if !defined _@GUARD_PREFIX@_SYS_SOCKET_H # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef socket # define socket socket_used_without_including_sys_socket_h # undef connect # define connect connect_used_without_including_sys_socket_h # undef accept # define accept accept_used_without_including_sys_socket_h # undef bind # define bind bind_used_without_including_sys_socket_h # undef getpeername # define getpeername getpeername_used_without_including_sys_socket_h # undef getsockname # define getsockname getsockname_used_without_including_sys_socket_h # undef getsockopt # define getsockopt getsockopt_used_without_including_sys_socket_h # undef listen # define listen listen_used_without_including_sys_socket_h # undef recv # define recv recv_used_without_including_sys_socket_h # undef send # define send send_used_without_including_sys_socket_h # undef recvfrom # define recvfrom recvfrom_used_without_including_sys_socket_h # undef sendto # define sendto sendto_used_without_including_sys_socket_h # undef setsockopt # define setsockopt setsockopt_used_without_including_sys_socket_h # undef shutdown # define shutdown shutdown_used_without_including_sys_socket_h # else _GL_WARN_ON_USE (socket, "socket() used without including "); _GL_WARN_ON_USE (connect, "connect() used without including "); _GL_WARN_ON_USE (accept, "accept() used without including "); _GL_WARN_ON_USE (bind, "bind() used without including "); _GL_WARN_ON_USE (getpeername, "getpeername() used without including "); _GL_WARN_ON_USE (getsockname, "getsockname() used without including "); _GL_WARN_ON_USE (getsockopt, "getsockopt() used without including "); _GL_WARN_ON_USE (listen, "listen() used without including "); _GL_WARN_ON_USE (recv, "recv() used without including "); _GL_WARN_ON_USE (send, "send() used without including "); _GL_WARN_ON_USE (recvfrom, "recvfrom() used without including "); _GL_WARN_ON_USE (sendto, "sendto() used without including "); _GL_WARN_ON_USE (setsockopt, "setsockopt() used without including "); _GL_WARN_ON_USE (shutdown, "shutdown() used without including "); # endif # endif # if !defined _@GUARD_PREFIX@_SYS_SELECT_H # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef select # define select select_used_without_including_sys_select_h # else _GL_WARN_ON_USE (select, "select() used without including "); # endif # endif #endif /* OS/2 EMX lacks these macros. */ #ifndef STDIN_FILENO # define STDIN_FILENO 0 #endif #ifndef STDOUT_FILENO # define STDOUT_FILENO 1 #endif #ifndef STDERR_FILENO # define STDERR_FILENO 2 #endif /* Ensure *_OK macros exist. */ #ifndef F_OK # define F_OK 0 # define X_OK 1 # define W_OK 2 # define R_OK 4 #endif /* Declare overridden functions. */ #if defined GNULIB_POSIXCHECK /* The access() function is a security risk. */ _GL_WARN_ON_USE (access, "the access function is a security risk - " "use the gnulib module faccessat instead"); #endif #if @GNULIB_CHDIR@ _GL_CXXALIAS_SYS (chdir, int, (const char *file) _GL_ARG_NONNULL ((1))); _GL_CXXALIASWARN (chdir); #elif defined GNULIB_POSIXCHECK # undef chdir # if HAVE_RAW_DECL_CHDIR _GL_WARN_ON_USE (chown, "chdir is not always in - " "use gnulib module chdir for portability"); # endif #endif #if @GNULIB_CHOWN@ /* Change the owner of FILE to UID (if UID is not -1) and the group of FILE to GID (if GID is not -1). Follow symbolic links. Return 0 if successful, otherwise -1 and errno set. See the POSIX:2008 specification . */ # if @REPLACE_DUP2@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define dup2 rpl_dup2 # endif _GL_FUNCDECL_RPL (dup2, int, (int oldfd, int newfd)); _GL_CXXALIAS_RPL (dup2, int, (int oldfd, int newfd)); # else # if !@HAVE_DUP2@ _GL_FUNCDECL_SYS (dup2, int, (int oldfd, int newfd)); # endif _GL_CXXALIAS_SYS (dup2, int, (int oldfd, int newfd)); # endif _GL_CXXALIASWARN (dup2); #elif defined GNULIB_POSIXCHECK # undef dup2 # if HAVE_RAW_DECL_DUP2 _GL_WARN_ON_USE (dup2, "dup2 is unportable - " "use gnulib module dup2 for portability"); # endif #endif #if @GNULIB_DUP3@ /* Copy the file descriptor OLDFD into file descriptor NEWFD, with the specified flags. The flags are a bitmask, possibly including O_CLOEXEC (defined in ) and O_TEXT, O_BINARY (defined in "binary-io.h"). Close NEWFD first if it is open. Return newfd if successful, otherwise -1 and errno set. See the Linux man page at . */ # if @HAVE_DUP3@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define dup3 rpl_dup3 # endif _GL_FUNCDECL_RPL (dup3, int, (int oldfd, int newfd, int flags)); _GL_CXXALIAS_RPL (dup3, int, (int oldfd, int newfd, int flags)); # else _GL_FUNCDECL_SYS (dup3, int, (int oldfd, int newfd, int flags)); _GL_CXXALIAS_SYS (dup3, int, (int oldfd, int newfd, int flags)); # endif _GL_CXXALIASWARN (dup3); #elif defined GNULIB_POSIXCHECK # undef dup3 # if HAVE_RAW_DECL_DUP3 _GL_WARN_ON_USE (dup3, "dup3 is unportable - " "use gnulib module dup3 for portability"); # endif #endif #if @GNULIB_ENVIRON@ # if !@HAVE_DECL_ENVIRON@ /* Set of environment variables and values. An array of strings of the form "VARIABLE=VALUE", terminated with a NULL. */ # if defined __APPLE__ && defined __MACH__ # include # if !TARGET_OS_IPHONE && !TARGET_IPHONE_SIMULATOR # define _GL_USE_CRT_EXTERNS # endif # endif # ifdef _GL_USE_CRT_EXTERNS # include # define environ (*_NSGetEnviron ()) # else # ifdef __cplusplus extern "C" { # endif extern char **environ; # ifdef __cplusplus } # endif # endif # endif #elif defined GNULIB_POSIXCHECK # if HAVE_RAW_DECL_ENVIRON _GL_UNISTD_INLINE char *** rpl_environ (void) { return &environ; } _GL_WARN_ON_USE (rpl_environ, "environ is unportable - " "use gnulib module environ for portability"); # undef environ # define environ (*rpl_environ ()) # endif #endif #if @GNULIB_EUIDACCESS@ /* Like access(), except that it uses the effective user id and group id of the current process. */ # if !@HAVE_EUIDACCESS@ _GL_FUNCDECL_SYS (euidaccess, int, (const char *filename, int mode) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (euidaccess, int, (const char *filename, int mode)); _GL_CXXALIASWARN (euidaccess); # if defined GNULIB_POSIXCHECK /* Like access(), this function is a security risk. */ _GL_WARN_ON_USE (euidaccess, "the euidaccess function is a security risk - " "use the gnulib module faccessat instead"); # endif #elif defined GNULIB_POSIXCHECK # undef euidaccess # if HAVE_RAW_DECL_EUIDACCESS _GL_WARN_ON_USE (euidaccess, "euidaccess is unportable - " "use gnulib module euidaccess for portability"); # endif #endif #if @GNULIB_FACCESSAT@ # if !@HAVE_FACCESSAT@ _GL_FUNCDECL_SYS (faccessat, int, (int fd, char const *file, int mode, int flag) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (faccessat, int, (int fd, char const *file, int mode, int flag)); _GL_CXXALIASWARN (faccessat); #elif defined GNULIB_POSIXCHECK # undef faccessat # if HAVE_RAW_DECL_FACCESSAT _GL_WARN_ON_USE (faccessat, "faccessat is not portable - " "use gnulib module faccessat for portability"); # endif #endif #if @GNULIB_FCHDIR@ /* Change the process' current working directory to the directory on which the given file descriptor is open. Return 0 if successful, otherwise -1 and errno set. See the POSIX:2008 specification . */ # if ! @HAVE_FCHDIR@ _GL_FUNCDECL_SYS (fchdir, int, (int /*fd*/)); /* Gnulib internal hooks needed to maintain the fchdir metadata. */ _GL_EXTERN_C int _gl_register_fd (int fd, const char *filename) _GL_ARG_NONNULL ((2)); _GL_EXTERN_C void _gl_unregister_fd (int fd); _GL_EXTERN_C int _gl_register_dup (int oldfd, int newfd); _GL_EXTERN_C const char *_gl_directory_name (int fd); # else # if !@HAVE_DECL_FCHDIR@ _GL_FUNCDECL_SYS (fchdir, int, (int /*fd*/)); # endif # endif _GL_CXXALIAS_SYS (fchdir, int, (int /*fd*/)); _GL_CXXALIASWARN (fchdir); #elif defined GNULIB_POSIXCHECK # undef fchdir # if HAVE_RAW_DECL_FCHDIR _GL_WARN_ON_USE (fchdir, "fchdir is unportable - " "use gnulib module fchdir for portability"); # endif #endif #if @GNULIB_FCHOWNAT@ # if @REPLACE_FCHOWNAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fchownat # define fchownat rpl_fchownat # endif _GL_FUNCDECL_RPL (fchownat, int, (int fd, char const *file, uid_t owner, gid_t group, int flag) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (fchownat, int, (int fd, char const *file, uid_t owner, gid_t group, int flag)); # else # if !@HAVE_FCHOWNAT@ _GL_FUNCDECL_SYS (fchownat, int, (int fd, char const *file, uid_t owner, gid_t group, int flag) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (fchownat, int, (int fd, char const *file, uid_t owner, gid_t group, int flag)); # endif _GL_CXXALIASWARN (fchownat); #elif defined GNULIB_POSIXCHECK # undef fchownat # if HAVE_RAW_DECL_FCHOWNAT _GL_WARN_ON_USE (fchownat, "fchownat is not portable - " "use gnulib module openat for portability"); # endif #endif #if @GNULIB_FDATASYNC@ /* Synchronize changes to a file. Return 0 if successful, otherwise -1 and errno set. See POSIX:2008 specification . */ # if !@HAVE_FDATASYNC@ || !@HAVE_DECL_FDATASYNC@ _GL_FUNCDECL_SYS (fdatasync, int, (int fd)); # endif _GL_CXXALIAS_SYS (fdatasync, int, (int fd)); _GL_CXXALIASWARN (fdatasync); #elif defined GNULIB_POSIXCHECK # undef fdatasync # if HAVE_RAW_DECL_FDATASYNC _GL_WARN_ON_USE (fdatasync, "fdatasync is unportable - " "use gnulib module fdatasync for portability"); # endif #endif #if @GNULIB_FSYNC@ /* Synchronize changes, including metadata, to a file. Return 0 if successful, otherwise -1 and errno set. See POSIX:2008 specification . */ # if !@HAVE_FSYNC@ _GL_FUNCDECL_SYS (fsync, int, (int fd)); # endif _GL_CXXALIAS_SYS (fsync, int, (int fd)); _GL_CXXALIASWARN (fsync); #elif defined GNULIB_POSIXCHECK # undef fsync # if HAVE_RAW_DECL_FSYNC _GL_WARN_ON_USE (fsync, "fsync is unportable - " "use gnulib module fsync for portability"); # endif #endif #if @GNULIB_FTRUNCATE@ /* Change the size of the file to which FD is opened to become equal to LENGTH. Return 0 if successful, otherwise -1 and errno set. See the POSIX:2008 specification . */ # if @REPLACE_FTRUNCATE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ftruncate # define ftruncate rpl_ftruncate # endif _GL_FUNCDECL_RPL (ftruncate, int, (int fd, off_t length)); _GL_CXXALIAS_RPL (ftruncate, int, (int fd, off_t length)); # else # if !@HAVE_FTRUNCATE@ _GL_FUNCDECL_SYS (ftruncate, int, (int fd, off_t length)); # endif _GL_CXXALIAS_SYS (ftruncate, int, (int fd, off_t length)); # endif _GL_CXXALIASWARN (ftruncate); #elif defined GNULIB_POSIXCHECK # undef ftruncate # if HAVE_RAW_DECL_FTRUNCATE _GL_WARN_ON_USE (ftruncate, "ftruncate is unportable - " "use gnulib module ftruncate for portability"); # endif #endif #if @GNULIB_GETCWD@ /* Get the name of the current working directory, and put it in SIZE bytes of BUF. Return BUF if successful, or NULL if the directory couldn't be determined or SIZE was too small. See the POSIX:2008 specification . Additionally, the gnulib module 'getcwd' guarantees the following GNU extension: If BUF is NULL, an array is allocated with 'malloc'; the array is SIZE bytes long, unless SIZE == 0, in which case it is as big as necessary. */ # if @REPLACE_GETCWD@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define getcwd rpl_getcwd # endif _GL_FUNCDECL_RPL (getcwd, char *, (char *buf, size_t size)); _GL_CXXALIAS_RPL (getcwd, char *, (char *buf, size_t size)); # else /* Need to cast, because on mingw, the second parameter is int size. */ _GL_CXXALIAS_SYS_CAST (getcwd, char *, (char *buf, size_t size)); # endif _GL_CXXALIASWARN (getcwd); #elif defined GNULIB_POSIXCHECK # undef getcwd # if HAVE_RAW_DECL_GETCWD _GL_WARN_ON_USE (getcwd, "getcwd is unportable - " "use gnulib module getcwd for portability"); # endif #endif #if @GNULIB_GETDOMAINNAME@ /* Return the NIS domain name of the machine. WARNING! The NIS domain name is unrelated to the fully qualified host name of the machine. It is also unrelated to email addresses. WARNING! The NIS domain name is usually the empty string or "(none)" when not using NIS. Put up to LEN bytes of the NIS domain name into NAME. Null terminate it if the name is shorter than LEN. If the NIS domain name is longer than LEN, set errno = EINVAL and return -1. Return 0 if successful, otherwise set errno and return -1. */ # if @REPLACE_GETDOMAINNAME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getdomainname # define getdomainname rpl_getdomainname # endif _GL_FUNCDECL_RPL (getdomainname, int, (char *name, size_t len) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (getdomainname, int, (char *name, size_t len)); # else # if !@HAVE_DECL_GETDOMAINNAME@ _GL_FUNCDECL_SYS (getdomainname, int, (char *name, size_t len) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (getdomainname, int, (char *name, size_t len)); # endif _GL_CXXALIASWARN (getdomainname); #elif defined GNULIB_POSIXCHECK # undef getdomainname # if HAVE_RAW_DECL_GETDOMAINNAME _GL_WARN_ON_USE (getdomainname, "getdomainname is unportable - " "use gnulib module getdomainname for portability"); # endif #endif #if @GNULIB_GETDTABLESIZE@ /* Return the maximum number of file descriptors in the current process. In POSIX, this is same as sysconf (_SC_OPEN_MAX). */ # if @REPLACE_GETDTABLESIZE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getdtablesize # define getdtablesize rpl_getdtablesize # endif _GL_FUNCDECL_RPL (getdtablesize, int, (void)); _GL_CXXALIAS_RPL (getdtablesize, int, (void)); # else # if !@HAVE_GETDTABLESIZE@ _GL_FUNCDECL_SYS (getdtablesize, int, (void)); # endif _GL_CXXALIAS_SYS (getdtablesize, int, (void)); # endif _GL_CXXALIASWARN (getdtablesize); #elif defined GNULIB_POSIXCHECK # undef getdtablesize # if HAVE_RAW_DECL_GETDTABLESIZE _GL_WARN_ON_USE (getdtablesize, "getdtablesize is unportable - " "use gnulib module getdtablesize for portability"); # endif #endif #if @GNULIB_GETGROUPS@ /* Return the supplemental groups that the current process belongs to. It is unspecified whether the effective group id is in the list. If N is 0, return the group count; otherwise, N describes how many entries are available in GROUPS. Return -1 and set errno if N is not 0 and not large enough. Fails with ENOSYS on some systems. */ # if @REPLACE_GETGROUPS@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getgroups # define getgroups rpl_getgroups # endif _GL_FUNCDECL_RPL (getgroups, int, (int n, gid_t *groups)); _GL_CXXALIAS_RPL (getgroups, int, (int n, gid_t *groups)); # else # if !@HAVE_GETGROUPS@ _GL_FUNCDECL_SYS (getgroups, int, (int n, gid_t *groups)); # endif _GL_CXXALIAS_SYS (getgroups, int, (int n, gid_t *groups)); # endif _GL_CXXALIASWARN (getgroups); #elif defined GNULIB_POSIXCHECK # undef getgroups # if HAVE_RAW_DECL_GETGROUPS _GL_WARN_ON_USE (getgroups, "getgroups is unportable - " "use gnulib module getgroups for portability"); # endif #endif #if @GNULIB_GETHOSTNAME@ /* Return the standard host name of the machine. WARNING! The host name may or may not be fully qualified. Put up to LEN bytes of the host name into NAME. Null terminate it if the name is shorter than LEN. If the host name is longer than LEN, set errno = EINVAL and return -1. Return 0 if successful, otherwise set errno and return -1. */ # if @UNISTD_H_HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef gethostname # define gethostname rpl_gethostname # endif _GL_FUNCDECL_RPL (gethostname, int, (char *name, size_t len) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (gethostname, int, (char *name, size_t len)); # else # if !@HAVE_GETHOSTNAME@ _GL_FUNCDECL_SYS (gethostname, int, (char *name, size_t len) _GL_ARG_NONNULL ((1))); # endif /* Need to cast, because on Solaris 10 and OSF/1 5.1 systems, the second parameter is int len. */ _GL_CXXALIAS_SYS_CAST (gethostname, int, (char *name, size_t len)); # endif _GL_CXXALIASWARN (gethostname); #elif @UNISTD_H_HAVE_WINSOCK2_H@ # undef gethostname # define gethostname gethostname_used_without_requesting_gnulib_module_gethostname #elif defined GNULIB_POSIXCHECK # undef gethostname # if HAVE_RAW_DECL_GETHOSTNAME _GL_WARN_ON_USE (gethostname, "gethostname is unportable - " "use gnulib module gethostname for portability"); # endif #endif #if @GNULIB_GETLOGIN@ /* Returns the user's login name, or NULL if it cannot be found. Upon error, returns NULL with errno set. See . Most programs don't need to use this function, because the information is available through environment variables: ${LOGNAME-$USER} on Unix platforms, $USERNAME on native Windows platforms. */ # if !@HAVE_GETLOGIN@ _GL_FUNCDECL_SYS (getlogin, char *, (void)); # endif _GL_CXXALIAS_SYS (getlogin, char *, (void)); _GL_CXXALIASWARN (getlogin); #elif defined GNULIB_POSIXCHECK # undef getlogin # if HAVE_RAW_DECL_GETLOGIN _GL_WARN_ON_USE (getlogin, "getlogin is unportable - " "use gnulib module getlogin for portability"); # endif #endif #if @GNULIB_GETLOGIN_R@ /* Copies the user's login name to NAME. The array pointed to by NAME has room for SIZE bytes. Returns 0 if successful. Upon error, an error number is returned, or -1 in the case that the login name cannot be found but no specific error is provided (this case is hopefully rare but is left open by the POSIX spec). See . Most programs don't need to use this function, because the information is available through environment variables: ${LOGNAME-$USER} on Unix platforms, $USERNAME on native Windows platforms. */ # if @REPLACE_GETLOGIN_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define getlogin_r rpl_getlogin_r # endif _GL_FUNCDECL_RPL (getlogin_r, int, (char *name, size_t size) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (getlogin_r, int, (char *name, size_t size)); # else # if !@HAVE_DECL_GETLOGIN_R@ _GL_FUNCDECL_SYS (getlogin_r, int, (char *name, size_t size) _GL_ARG_NONNULL ((1))); # endif /* Need to cast, because on Solaris 10 systems, the second argument is int size. */ _GL_CXXALIAS_SYS_CAST (getlogin_r, int, (char *name, size_t size)); # endif _GL_CXXALIASWARN (getlogin_r); #elif defined GNULIB_POSIXCHECK # undef getlogin_r # if HAVE_RAW_DECL_GETLOGIN_R _GL_WARN_ON_USE (getlogin_r, "getlogin_r is unportable - " "use gnulib module getlogin_r for portability"); # endif #endif #if @GNULIB_GETPAGESIZE@ # if @REPLACE_GETPAGESIZE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define getpagesize rpl_getpagesize # endif _GL_FUNCDECL_RPL (getpagesize, int, (void)); _GL_CXXALIAS_RPL (getpagesize, int, (void)); # else # if !@HAVE_GETPAGESIZE@ # if !defined getpagesize /* This is for POSIX systems. */ # if !defined _gl_getpagesize && defined _SC_PAGESIZE # if ! (defined __VMS && __VMS_VER < 70000000) # define _gl_getpagesize() sysconf (_SC_PAGESIZE) # endif # endif /* This is for older VMS. */ # if !defined _gl_getpagesize && defined __VMS # ifdef __ALPHA # define _gl_getpagesize() 8192 # else # define _gl_getpagesize() 512 # endif # endif /* This is for BeOS. */ # if !defined _gl_getpagesize && @HAVE_OS_H@ # include # if defined B_PAGE_SIZE # define _gl_getpagesize() B_PAGE_SIZE # endif # endif /* This is for AmigaOS4.0. */ # if !defined _gl_getpagesize && defined __amigaos4__ # define _gl_getpagesize() 2048 # endif /* This is for older Unix systems. */ # if !defined _gl_getpagesize && @HAVE_SYS_PARAM_H@ # include # ifdef EXEC_PAGESIZE # define _gl_getpagesize() EXEC_PAGESIZE # else # ifdef NBPG # ifndef CLSIZE # define CLSIZE 1 # endif # define _gl_getpagesize() (NBPG * CLSIZE) # else # ifdef NBPC # define _gl_getpagesize() NBPC # endif # endif # endif # endif # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define getpagesize() _gl_getpagesize () # else # if !GNULIB_defined_getpagesize_function _GL_UNISTD_INLINE int getpagesize () { return _gl_getpagesize (); } # define GNULIB_defined_getpagesize_function 1 # endif # endif # endif # endif /* Need to cast, because on Cygwin 1.5.x systems, the return type is size_t. */ _GL_CXXALIAS_SYS_CAST (getpagesize, int, (void)); # endif # if @HAVE_DECL_GETPAGESIZE@ _GL_CXXALIASWARN (getpagesize); # endif #elif defined GNULIB_POSIXCHECK # undef getpagesize # if HAVE_RAW_DECL_GETPAGESIZE _GL_WARN_ON_USE (getpagesize, "getpagesize is unportable - " "use gnulib module getpagesize for portability"); # endif #endif #if @GNULIB_GETUSERSHELL@ /* Return the next valid login shell on the system, or NULL when the end of the list has been reached. */ # if !@HAVE_DECL_GETUSERSHELL@ _GL_FUNCDECL_SYS (getusershell, char *, (void)); # endif _GL_CXXALIAS_SYS (getusershell, char *, (void)); _GL_CXXALIASWARN (getusershell); #elif defined GNULIB_POSIXCHECK # undef getusershell # if HAVE_RAW_DECL_GETUSERSHELL _GL_WARN_ON_USE (getusershell, "getusershell is unportable - " "use gnulib module getusershell for portability"); # endif #endif #if @GNULIB_GETUSERSHELL@ /* Rewind to pointer that is advanced at each getusershell() call. */ # if !@HAVE_DECL_GETUSERSHELL@ _GL_FUNCDECL_SYS (setusershell, void, (void)); # endif _GL_CXXALIAS_SYS (setusershell, void, (void)); _GL_CXXALIASWARN (setusershell); #elif defined GNULIB_POSIXCHECK # undef setusershell # if HAVE_RAW_DECL_SETUSERSHELL _GL_WARN_ON_USE (setusershell, "setusershell is unportable - " "use gnulib module getusershell for portability"); # endif #endif #if @GNULIB_GETUSERSHELL@ /* Free the pointer that is advanced at each getusershell() call and associated resources. */ # if !@HAVE_DECL_GETUSERSHELL@ _GL_FUNCDECL_SYS (endusershell, void, (void)); # endif _GL_CXXALIAS_SYS (endusershell, void, (void)); _GL_CXXALIASWARN (endusershell); #elif defined GNULIB_POSIXCHECK # undef endusershell # if HAVE_RAW_DECL_ENDUSERSHELL _GL_WARN_ON_USE (endusershell, "endusershell is unportable - " "use gnulib module getusershell for portability"); # endif #endif #if @GNULIB_GROUP_MEMBER@ /* Determine whether group id is in calling user's group list. */ # if !@HAVE_GROUP_MEMBER@ _GL_FUNCDECL_SYS (group_member, int, (gid_t gid)); # endif _GL_CXXALIAS_SYS (group_member, int, (gid_t gid)); _GL_CXXALIASWARN (group_member); #elif defined GNULIB_POSIXCHECK # undef group_member # if HAVE_RAW_DECL_GROUP_MEMBER _GL_WARN_ON_USE (group_member, "group_member is unportable - " "use gnulib module group-member for portability"); # endif #endif #if @GNULIB_ISATTY@ # if @REPLACE_ISATTY@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef isatty # define isatty rpl_isatty # endif _GL_FUNCDECL_RPL (isatty, int, (int fd)); _GL_CXXALIAS_RPL (isatty, int, (int fd)); # else _GL_CXXALIAS_SYS (isatty, int, (int fd)); # endif _GL_CXXALIASWARN (isatty); #elif defined GNULIB_POSIXCHECK # undef isatty # if HAVE_RAW_DECL_ISATTY _GL_WARN_ON_USE (isatty, "isatty has portability problems on native Windows - " "use gnulib module isatty for portability"); # endif #endif #if @GNULIB_LCHOWN@ /* Change the owner of FILE to UID (if UID is not -1) and the group of FILE to GID (if GID is not -1). Do not follow symbolic links. Return 0 if successful, otherwise -1 and errno set. See the POSIX:2008 specification . */ # if @REPLACE_LCHOWN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef lchown # define lchown rpl_lchown # endif _GL_FUNCDECL_RPL (lchown, int, (char const *file, uid_t owner, gid_t group) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (lchown, int, (char const *file, uid_t owner, gid_t group)); # else # if !@HAVE_LCHOWN@ _GL_FUNCDECL_SYS (lchown, int, (char const *file, uid_t owner, gid_t group) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (lchown, int, (char const *file, uid_t owner, gid_t group)); # endif _GL_CXXALIASWARN (lchown); #elif defined GNULIB_POSIXCHECK # undef lchown # if HAVE_RAW_DECL_LCHOWN _GL_WARN_ON_USE (lchown, "lchown is unportable to pre-POSIX.1-2001 systems - " "use gnulib module lchown for portability"); # endif #endif #if @GNULIB_LINK@ /* Create a new hard link for an existing file. Return 0 if successful, otherwise -1 and errno set. See POSIX:2008 specification . */ # if @REPLACE_LINK@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define link rpl_link # endif _GL_FUNCDECL_RPL (link, int, (const char *path1, const char *path2) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (link, int, (const char *path1, const char *path2)); # else # if !@HAVE_LINK@ _GL_FUNCDECL_SYS (link, int, (const char *path1, const char *path2) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (link, int, (const char *path1, const char *path2)); # endif _GL_CXXALIASWARN (link); #elif defined GNULIB_POSIXCHECK # undef link # if HAVE_RAW_DECL_LINK _GL_WARN_ON_USE (link, "link is unportable - " "use gnulib module link for portability"); # endif #endif #if @GNULIB_LINKAT@ /* Create a new hard link for an existing file, relative to two directories. FLAG controls whether symlinks are followed. Return 0 if successful, otherwise -1 and errno set. */ # if @REPLACE_LINKAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef linkat # define linkat rpl_linkat # endif _GL_FUNCDECL_RPL (linkat, int, (int fd1, const char *path1, int fd2, const char *path2, int flag) _GL_ARG_NONNULL ((2, 4))); _GL_CXXALIAS_RPL (linkat, int, (int fd1, const char *path1, int fd2, const char *path2, int flag)); # else # if !@HAVE_LINKAT@ _GL_FUNCDECL_SYS (linkat, int, (int fd1, const char *path1, int fd2, const char *path2, int flag) _GL_ARG_NONNULL ((2, 4))); # endif _GL_CXXALIAS_SYS (linkat, int, (int fd1, const char *path1, int fd2, const char *path2, int flag)); # endif _GL_CXXALIASWARN (linkat); #elif defined GNULIB_POSIXCHECK # undef linkat # if HAVE_RAW_DECL_LINKAT _GL_WARN_ON_USE (linkat, "linkat is unportable - " "use gnulib module linkat for portability"); # endif #endif #if @GNULIB_LSEEK@ /* Set the offset of FD relative to SEEK_SET, SEEK_CUR, or SEEK_END. Return the new offset if successful, otherwise -1 and errno set. See the POSIX:2008 specification . */ # if @REPLACE_LSEEK@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define lseek rpl_lseek # endif _GL_FUNCDECL_RPL (lseek, off_t, (int fd, off_t offset, int whence)); _GL_CXXALIAS_RPL (lseek, off_t, (int fd, off_t offset, int whence)); # else _GL_CXXALIAS_SYS (lseek, off_t, (int fd, off_t offset, int whence)); # endif _GL_CXXALIASWARN (lseek); #elif defined GNULIB_POSIXCHECK # undef lseek # if HAVE_RAW_DECL_LSEEK _GL_WARN_ON_USE (lseek, "lseek does not fail with ESPIPE on pipes on some " "systems - use gnulib module lseek for portability"); # endif #endif #if @GNULIB_PIPE@ /* Create a pipe, defaulting to O_BINARY mode. Store the read-end as fd[0] and the write-end as fd[1]. Return 0 upon success, or -1 with errno set upon failure. */ # if !@HAVE_PIPE@ _GL_FUNCDECL_SYS (pipe, int, (int fd[2]) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (pipe, int, (int fd[2])); _GL_CXXALIASWARN (pipe); #elif defined GNULIB_POSIXCHECK # undef pipe # if HAVE_RAW_DECL_PIPE _GL_WARN_ON_USE (pipe, "pipe is unportable - " "use gnulib module pipe-posix for portability"); # endif #endif #if @GNULIB_PIPE2@ /* Create a pipe, applying the given flags when opening the read-end of the pipe and the write-end of the pipe. The flags are a bitmask, possibly including O_CLOEXEC (defined in ) and O_TEXT, O_BINARY (defined in "binary-io.h"). Store the read-end as fd[0] and the write-end as fd[1]. Return 0 upon success, or -1 with errno set upon failure. See also the Linux man page at . */ # if @HAVE_PIPE2@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define pipe2 rpl_pipe2 # endif _GL_FUNCDECL_RPL (pipe2, int, (int fd[2], int flags) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (pipe2, int, (int fd[2], int flags)); # else _GL_FUNCDECL_SYS (pipe2, int, (int fd[2], int flags) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_SYS (pipe2, int, (int fd[2], int flags)); # endif _GL_CXXALIASWARN (pipe2); #elif defined GNULIB_POSIXCHECK # undef pipe2 # if HAVE_RAW_DECL_PIPE2 _GL_WARN_ON_USE (pipe2, "pipe2 is unportable - " "use gnulib module pipe2 for portability"); # endif #endif #if @GNULIB_PREAD@ /* Read at most BUFSIZE bytes from FD into BUF, starting at OFFSET. Return the number of bytes placed into BUF if successful, otherwise set errno and return -1. 0 indicates EOF. See the POSIX:2008 specification . */ # if @REPLACE_PREAD@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef pread # define pread rpl_pread # endif _GL_FUNCDECL_RPL (pread, ssize_t, (int fd, void *buf, size_t bufsize, off_t offset) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (pread, ssize_t, (int fd, void *buf, size_t bufsize, off_t offset)); # else # if !@HAVE_PREAD@ _GL_FUNCDECL_SYS (pread, ssize_t, (int fd, void *buf, size_t bufsize, off_t offset) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (pread, ssize_t, (int fd, void *buf, size_t bufsize, off_t offset)); # endif _GL_CXXALIASWARN (pread); #elif defined GNULIB_POSIXCHECK # undef pread # if HAVE_RAW_DECL_PREAD _GL_WARN_ON_USE (pread, "pread is unportable - " "use gnulib module pread for portability"); # endif #endif #if @GNULIB_PWRITE@ /* Write at most BUFSIZE bytes from BUF into FD, starting at OFFSET. Return the number of bytes written if successful, otherwise set errno and return -1. 0 indicates nothing written. See the POSIX:2008 specification . */ # if @REPLACE_PWRITE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef pwrite # define pwrite rpl_pwrite # endif _GL_FUNCDECL_RPL (pwrite, ssize_t, (int fd, const void *buf, size_t bufsize, off_t offset) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (pwrite, ssize_t, (int fd, const void *buf, size_t bufsize, off_t offset)); # else # if !@HAVE_PWRITE@ _GL_FUNCDECL_SYS (pwrite, ssize_t, (int fd, const void *buf, size_t bufsize, off_t offset) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (pwrite, ssize_t, (int fd, const void *buf, size_t bufsize, off_t offset)); # endif _GL_CXXALIASWARN (pwrite); #elif defined GNULIB_POSIXCHECK # undef pwrite # if HAVE_RAW_DECL_PWRITE _GL_WARN_ON_USE (pwrite, "pwrite is unportable - " "use gnulib module pwrite for portability"); # endif #endif #if @GNULIB_READ@ /* Read up to COUNT bytes from file descriptor FD into the buffer starting at BUF. See the POSIX:2008 specification . */ # if @REPLACE_READ@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef read # define read rpl_read # endif _GL_FUNCDECL_RPL (read, ssize_t, (int fd, void *buf, size_t count) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (read, ssize_t, (int fd, void *buf, size_t count)); # else /* Need to cast, because on mingw, the third parameter is unsigned int count and the return type is 'int'. */ _GL_CXXALIAS_SYS_CAST (read, ssize_t, (int fd, void *buf, size_t count)); # endif _GL_CXXALIASWARN (read); #endif #if @GNULIB_READLINK@ /* Read the contents of the symbolic link FILE and place the first BUFSIZE bytes of it into BUF. Return the number of bytes placed into BUF if successful, otherwise -1 and errno set. See the POSIX:2008 specification . */ # if @REPLACE_READLINK@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define readlink rpl_readlink # endif _GL_FUNCDECL_RPL (readlink, ssize_t, (const char *file, char *buf, size_t bufsize) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (readlink, ssize_t, (const char *file, char *buf, size_t bufsize)); # else # if !@HAVE_READLINK@ _GL_FUNCDECL_SYS (readlink, ssize_t, (const char *file, char *buf, size_t bufsize) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (readlink, ssize_t, (const char *file, char *buf, size_t bufsize)); # endif _GL_CXXALIASWARN (readlink); #elif defined GNULIB_POSIXCHECK # undef readlink # if HAVE_RAW_DECL_READLINK _GL_WARN_ON_USE (readlink, "readlink is unportable - " "use gnulib module readlink for portability"); # endif #endif #if @GNULIB_READLINKAT@ # if @REPLACE_READLINKAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define readlinkat rpl_readlinkat # endif _GL_FUNCDECL_RPL (readlinkat, ssize_t, (int fd, char const *file, char *buf, size_t len) _GL_ARG_NONNULL ((2, 3))); _GL_CXXALIAS_RPL (readlinkat, ssize_t, (int fd, char const *file, char *buf, size_t len)); # else # if !@HAVE_READLINKAT@ _GL_FUNCDECL_SYS (readlinkat, ssize_t, (int fd, char const *file, char *buf, size_t len) _GL_ARG_NONNULL ((2, 3))); # endif _GL_CXXALIAS_SYS (readlinkat, ssize_t, (int fd, char const *file, char *buf, size_t len)); # endif _GL_CXXALIASWARN (readlinkat); #elif defined GNULIB_POSIXCHECK # undef readlinkat # if HAVE_RAW_DECL_READLINKAT _GL_WARN_ON_USE (readlinkat, "readlinkat is not portable - " "use gnulib module readlinkat for portability"); # endif #endif #if @GNULIB_RMDIR@ /* Remove the directory DIR. */ # if @REPLACE_RMDIR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define rmdir rpl_rmdir # endif _GL_FUNCDECL_RPL (rmdir, int, (char const *name) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (rmdir, int, (char const *name)); # else _GL_CXXALIAS_SYS (rmdir, int, (char const *name)); # endif _GL_CXXALIASWARN (rmdir); #elif defined GNULIB_POSIXCHECK # undef rmdir # if HAVE_RAW_DECL_RMDIR _GL_WARN_ON_USE (rmdir, "rmdir is unportable - " "use gnulib module rmdir for portability"); # endif #endif #if @GNULIB_SETHOSTNAME@ /* Set the host name of the machine. The host name may or may not be fully qualified. Put LEN bytes of NAME into the host name. Return 0 if successful, otherwise, set errno and return -1. Platforms with no ability to set the hostname return -1 and set errno = ENOSYS. */ # if !@HAVE_SETHOSTNAME@ || !@HAVE_DECL_SETHOSTNAME@ _GL_FUNCDECL_SYS (sethostname, int, (const char *name, size_t len) _GL_ARG_NONNULL ((1))); # endif /* Need to cast, because on Solaris 11 2011-10, Mac OS X 10.5, IRIX 6.5 and FreeBSD 6.4 the second parameter is int. On Solaris 11 2011-10, the first parameter is not const. */ _GL_CXXALIAS_SYS_CAST (sethostname, int, (const char *name, size_t len)); _GL_CXXALIASWARN (sethostname); #elif defined GNULIB_POSIXCHECK # undef sethostname # if HAVE_RAW_DECL_SETHOSTNAME _GL_WARN_ON_USE (sethostname, "sethostname is unportable - " "use gnulib module sethostname for portability"); # endif #endif #if @GNULIB_SLEEP@ /* Pause the execution of the current thread for N seconds. Returns the number of seconds left to sleep. See the POSIX:2008 specification . */ # if @REPLACE_SLEEP@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef sleep # define sleep rpl_sleep # endif _GL_FUNCDECL_RPL (sleep, unsigned int, (unsigned int n)); _GL_CXXALIAS_RPL (sleep, unsigned int, (unsigned int n)); # else # if !@HAVE_SLEEP@ _GL_FUNCDECL_SYS (sleep, unsigned int, (unsigned int n)); # endif _GL_CXXALIAS_SYS (sleep, unsigned int, (unsigned int n)); # endif _GL_CXXALIASWARN (sleep); #elif defined GNULIB_POSIXCHECK # undef sleep # if HAVE_RAW_DECL_SLEEP _GL_WARN_ON_USE (sleep, "sleep is unportable - " "use gnulib module sleep for portability"); # endif #endif #if @GNULIB_SYMLINK@ # if @REPLACE_SYMLINK@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef symlink # define symlink rpl_symlink # endif _GL_FUNCDECL_RPL (symlink, int, (char const *contents, char const *file) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (symlink, int, (char const *contents, char const *file)); # else # if !@HAVE_SYMLINK@ _GL_FUNCDECL_SYS (symlink, int, (char const *contents, char const *file) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (symlink, int, (char const *contents, char const *file)); # endif _GL_CXXALIASWARN (symlink); #elif defined GNULIB_POSIXCHECK # undef symlink # if HAVE_RAW_DECL_SYMLINK _GL_WARN_ON_USE (symlink, "symlink is not portable - " "use gnulib module symlink for portability"); # endif #endif #if @GNULIB_SYMLINKAT@ # if @REPLACE_SYMLINKAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef symlinkat # define symlinkat rpl_symlinkat # endif _GL_FUNCDECL_RPL (symlinkat, int, (char const *contents, int fd, char const *file) _GL_ARG_NONNULL ((1, 3))); _GL_CXXALIAS_RPL (symlinkat, int, (char const *contents, int fd, char const *file)); # else # if !@HAVE_SYMLINKAT@ _GL_FUNCDECL_SYS (symlinkat, int, (char const *contents, int fd, char const *file) _GL_ARG_NONNULL ((1, 3))); # endif _GL_CXXALIAS_SYS (symlinkat, int, (char const *contents, int fd, char const *file)); # endif _GL_CXXALIASWARN (symlinkat); #elif defined GNULIB_POSIXCHECK # undef symlinkat # if HAVE_RAW_DECL_SYMLINKAT _GL_WARN_ON_USE (symlinkat, "symlinkat is not portable - " "use gnulib module symlinkat for portability"); # endif #endif #if @GNULIB_TTYNAME_R@ /* Store at most BUFLEN characters of the pathname of the terminal FD is open on in BUF. Return 0 on success, otherwise an error number. */ # if @REPLACE_TTYNAME_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ttyname_r # define ttyname_r rpl_ttyname_r # endif _GL_FUNCDECL_RPL (ttyname_r, int, (int fd, char *buf, size_t buflen) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (ttyname_r, int, (int fd, char *buf, size_t buflen)); # else # if !@HAVE_DECL_TTYNAME_R@ _GL_FUNCDECL_SYS (ttyname_r, int, (int fd, char *buf, size_t buflen) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (ttyname_r, int, (int fd, char *buf, size_t buflen)); # endif _GL_CXXALIASWARN (ttyname_r); #elif defined GNULIB_POSIXCHECK # undef ttyname_r # if HAVE_RAW_DECL_TTYNAME_R _GL_WARN_ON_USE (ttyname_r, "ttyname_r is not portable - " "use gnulib module ttyname_r for portability"); # endif #endif #if @GNULIB_UNLINK@ # if @REPLACE_UNLINK@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef unlink # define unlink rpl_unlink # endif _GL_FUNCDECL_RPL (unlink, int, (char const *file) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (unlink, int, (char const *file)); # else _GL_CXXALIAS_SYS (unlink, int, (char const *file)); # endif _GL_CXXALIASWARN (unlink); #elif defined GNULIB_POSIXCHECK # undef unlink # if HAVE_RAW_DECL_UNLINK _GL_WARN_ON_USE (unlink, "unlink is not portable - " "use gnulib module unlink for portability"); # endif #endif #if @GNULIB_UNLINKAT@ # if @REPLACE_UNLINKAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef unlinkat # define unlinkat rpl_unlinkat # endif _GL_FUNCDECL_RPL (unlinkat, int, (int fd, char const *file, int flag) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (unlinkat, int, (int fd, char const *file, int flag)); # else # if !@HAVE_UNLINKAT@ _GL_FUNCDECL_SYS (unlinkat, int, (int fd, char const *file, int flag) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (unlinkat, int, (int fd, char const *file, int flag)); # endif _GL_CXXALIASWARN (unlinkat); #elif defined GNULIB_POSIXCHECK # undef unlinkat # if HAVE_RAW_DECL_UNLINKAT _GL_WARN_ON_USE (unlinkat, "unlinkat is not portable - " "use gnulib module openat for portability"); # endif #endif #if @GNULIB_USLEEP@ /* Pause the execution of the current thread for N microseconds. Returns 0 on completion, or -1 on range error. See the POSIX:2001 specification . */ # if @REPLACE_USLEEP@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef usleep # define usleep rpl_usleep # endif _GL_FUNCDECL_RPL (usleep, int, (useconds_t n)); _GL_CXXALIAS_RPL (usleep, int, (useconds_t n)); # else # if !@HAVE_USLEEP@ _GL_FUNCDECL_SYS (usleep, int, (useconds_t n)); # endif _GL_CXXALIAS_SYS (usleep, int, (useconds_t n)); # endif _GL_CXXALIASWARN (usleep); #elif defined GNULIB_POSIXCHECK # undef usleep # if HAVE_RAW_DECL_USLEEP _GL_WARN_ON_USE (usleep, "usleep is unportable - " "use gnulib module usleep for portability"); # endif #endif #if @GNULIB_WRITE@ /* Write up to COUNT bytes starting at BUF to file descriptor FD. See the POSIX:2008 specification . */ # if @REPLACE_WRITE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef write # define write rpl_write # endif _GL_FUNCDECL_RPL (write, ssize_t, (int fd, const void *buf, size_t count) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (write, ssize_t, (int fd, const void *buf, size_t count)); # else /* Need to cast, because on mingw, the third parameter is unsigned int count and the return type is 'int'. */ _GL_CXXALIAS_SYS_CAST (write, ssize_t, (int fd, const void *buf, size_t count)); # endif _GL_CXXALIASWARN (write); #endif _GL_INLINE_HEADER_END #endif /* _@GUARD_PREFIX@_UNISTD_H */ #endif /* _GL_INCLUDING_UNISTD_H */ #endif /* _@GUARD_PREFIX@_UNISTD_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/sysexits.in.h0000644000175000017500000000366713004436754017064 00000000000000/* exit() exit codes for some BSD system programs. Copyright (C) 2003, 2006-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Simon Josefsson based on sysexits(3) man page */ #ifndef _@GUARD_PREFIX@_SYSEXITS_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if @HAVE_SYSEXITS_H@ /* IRIX 6.5 has an that defines a macro EX_OK with a nonzero value. Override it. See */ # ifdef __sgi # include # undef EX_OK # endif /* The include_next requires a split double-inclusion guard. */ # @INCLUDE_NEXT@ @NEXT_SYSEXITS_H@ /* HP-UX 11 ends at EX_NOPERM. */ # ifndef EX_CONFIG # define EX_CONFIG 78 # endif #endif #ifndef _@GUARD_PREFIX@_SYSEXITS_H #define _@GUARD_PREFIX@_SYSEXITS_H #if !@HAVE_SYSEXITS_H@ # define EX_OK 0 /* same value as EXIT_SUCCESS */ # define EX_USAGE 64 # define EX_DATAERR 65 # define EX_NOINPUT 66 # define EX_NOUSER 67 # define EX_NOHOST 68 # define EX_UNAVAILABLE 69 # define EX_SOFTWARE 70 # define EX_OSERR 71 # define EX_OSFILE 72 # define EX_CANTCREAT 73 # define EX_IOERR 74 # define EX_TEMPFAIL 75 # define EX_PROTOCOL 76 # define EX_NOPERM 77 # define EX_CONFIG 78 #endif #endif /* _@GUARD_PREFIX@_SYSEXITS_H */ #endif /* _@GUARD_PREFIX@_SYSEXITS_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/sys_types.in.h0000644000175000017500000000330213004436754017215 00000000000000/* Provide a more complete sys/types.h. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #ifndef _@GUARD_PREFIX@_SYS_TYPES_H /* The include_next requires a split double-inclusion guard. */ # define _GL_INCLUDING_SYS_TYPES_H #@INCLUDE_NEXT@ @NEXT_SYS_TYPES_H@ # undef _GL_INCLUDING_SYS_TYPES_H #ifndef _@GUARD_PREFIX@_SYS_TYPES_H #define _@GUARD_PREFIX@_SYS_TYPES_H /* Override off_t if Large File Support is requested on native Windows. */ #if @WINDOWS_64_BIT_OFF_T@ /* Same as int64_t in . */ # if defined _MSC_VER # define off_t __int64 # else # define off_t long long int # endif /* Indicator, for gnulib internal purposes. */ # define _GL_WINDOWS_64_BIT_OFF_T 1 #endif /* MSVC 9 defines size_t in , not in . */ /* But avoid namespace pollution on glibc systems. */ #if ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) \ && ! defined __GLIBC__ # include #endif #endif /* _@GUARD_PREFIX@_SYS_TYPES_H */ #endif /* _@GUARD_PREFIX@_SYS_TYPES_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/strings.in.h0000644000175000017500000000765613004436754016664 00000000000000/* A substitute . Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _@GUARD_PREFIX@_STRINGS_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* Minix 3.1.8 has a bug: must be included before . But avoid namespace pollution on glibc systems. */ #if defined __minix && !defined __GLIBC__ # include #endif /* The include_next requires a split double-inclusion guard. */ #if @HAVE_STRINGS_H@ # @INCLUDE_NEXT@ @NEXT_STRINGS_H@ #endif #ifndef _@GUARD_PREFIX@_STRINGS_H #define _@GUARD_PREFIX@_STRINGS_H #if ! @HAVE_DECL_STRNCASECMP@ /* Get size_t. */ # include #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ #ifdef __cplusplus extern "C" { #endif /* Find the index of the least-significant set bit. */ #if @GNULIB_FFS@ # if !@HAVE_FFS@ _GL_FUNCDECL_SYS (ffs, int, (int i)); # endif _GL_CXXALIAS_SYS (ffs, int, (int i)); _GL_CXXALIASWARN (ffs); #elif defined GNULIB_POSIXCHECK # undef ffs # if HAVE_RAW_DECL_FFS _GL_WARN_ON_USE (ffs, "ffs is not portable - use the ffs module"); # endif #endif /* Compare strings S1 and S2, ignoring case, returning less than, equal to or greater than zero if S1 is lexicographically less than, equal to or greater than S2. Note: This function does not work in multibyte locales. */ #if ! @HAVE_STRCASECMP@ extern int strcasecmp (char const *s1, char const *s2) _GL_ARG_NONNULL ((1, 2)); #endif #if defined GNULIB_POSIXCHECK /* strcasecmp() does not work with multibyte strings: POSIX says that it operates on "strings", and "string" in POSIX is defined as a sequence of bytes, not of characters. */ # undef strcasecmp # if HAVE_RAW_DECL_STRCASECMP _GL_WARN_ON_USE (strcasecmp, "strcasecmp cannot work correctly on character " "strings in multibyte locales - " "use mbscasecmp if you care about " "internationalization, or use c_strcasecmp , " "gnulib module c-strcase) if you want a locale " "independent function"); # endif #endif /* Compare no more than N bytes of strings S1 and S2, ignoring case, returning less than, equal to or greater than zero if S1 is lexicographically less than, equal to or greater than S2. Note: This function cannot work correctly in multibyte locales. */ #if ! @HAVE_DECL_STRNCASECMP@ extern int strncasecmp (char const *s1, char const *s2, size_t n) _GL_ARG_NONNULL ((1, 2)); #endif #if defined GNULIB_POSIXCHECK /* strncasecmp() does not work with multibyte strings: POSIX says that it operates on "strings", and "string" in POSIX is defined as a sequence of bytes, not of characters. */ # undef strncasecmp # if HAVE_RAW_DECL_STRNCASECMP _GL_WARN_ON_USE (strncasecmp, "strncasecmp cannot work correctly on character " "strings in multibyte locales - " "use mbsncasecmp or mbspcasecmp if you care about " "internationalization, or use c_strncasecmp , " "gnulib module c-strcase) if you want a locale " "independent function"); # endif #endif #ifdef __cplusplus } #endif #endif /* _@GUARD_PREFIX@_STRING_H */ #endif /* _@GUARD_PREFIX@_STRING_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/string.in.h0000644000175000017500000011734413004436754016475 00000000000000/* A GNU-like . Copyright (C) 1995-1996, 2001-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if defined _GL_ALREADY_INCLUDING_STRING_H /* Special invocation convention: - On OS X/NetBSD we have a sequence of nested includes -> -> "string.h" In this situation system _chk variants due to -D_FORTIFY_SOURCE might be used after any replacements defined here. */ #@INCLUDE_NEXT@ @NEXT_STRING_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_STRING_H #define _GL_ALREADY_INCLUDING_STRING_H /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_STRING_H@ #undef _GL_ALREADY_INCLUDING_STRING_H #ifndef _@GUARD_PREFIX@_STRING_H #define _@GUARD_PREFIX@_STRING_H /* NetBSD 5.0 mis-defines NULL. */ #include /* MirBSD defines mbslen as a macro. */ #if @GNULIB_MBSLEN@ && defined __MirBSD__ # include #endif /* The __attribute__ feature is available in gcc versions 2.5 and later. The attribute __pure__ was added in gcc 2.96. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 96) # define _GL_ATTRIBUTE_PURE __attribute__ ((__pure__)) #else # define _GL_ATTRIBUTE_PURE /* empty */ #endif /* NetBSD 5.0 declares strsignal in , not in . */ /* But in any case avoid namespace pollution on glibc systems. */ #if (@GNULIB_STRSIGNAL@ || defined GNULIB_POSIXCHECK) && defined __NetBSD__ \ && ! defined __GLIBC__ # include #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Find the index of the least-significant set bit. */ #if @GNULIB_FFSL@ # if !@HAVE_FFSL@ _GL_FUNCDECL_SYS (ffsl, int, (long int i)); # endif _GL_CXXALIAS_SYS (ffsl, int, (long int i)); _GL_CXXALIASWARN (ffsl); #elif defined GNULIB_POSIXCHECK # undef ffsl # if HAVE_RAW_DECL_FFSL _GL_WARN_ON_USE (ffsl, "ffsl is not portable - use the ffsl module"); # endif #endif /* Find the index of the least-significant set bit. */ #if @GNULIB_FFSLL@ # if !@HAVE_FFSLL@ _GL_FUNCDECL_SYS (ffsll, int, (long long int i)); # endif _GL_CXXALIAS_SYS (ffsll, int, (long long int i)); _GL_CXXALIASWARN (ffsll); #elif defined GNULIB_POSIXCHECK # undef ffsll # if HAVE_RAW_DECL_FFSLL _GL_WARN_ON_USE (ffsll, "ffsll is not portable - use the ffsll module"); # endif #endif /* Return the first instance of C within N bytes of S, or NULL. */ #if @GNULIB_MEMCHR@ # if @REPLACE_MEMCHR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define memchr rpl_memchr # endif _GL_FUNCDECL_RPL (memchr, void *, (void const *__s, int __c, size_t __n) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (memchr, void *, (void const *__s, int __c, size_t __n)); # else # if ! @HAVE_MEMCHR@ _GL_FUNCDECL_SYS (memchr, void *, (void const *__s, int __c, size_t __n) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); # endif /* On some systems, this function is defined as an overloaded function: extern "C" { const void * std::memchr (const void *, int, size_t); } extern "C++" { void * std::memchr (void *, int, size_t); } */ _GL_CXXALIAS_SYS_CAST2 (memchr, void *, (void const *__s, int __c, size_t __n), void const *, (void const *__s, int __c, size_t __n)); # endif # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (memchr, void *, (void *__s, int __c, size_t __n)); _GL_CXXALIASWARN1 (memchr, void const *, (void const *__s, int __c, size_t __n)); # else _GL_CXXALIASWARN (memchr); # endif #elif defined GNULIB_POSIXCHECK # undef memchr /* Assume memchr is always declared. */ _GL_WARN_ON_USE (memchr, "memchr has platform-specific bugs - " "use gnulib module memchr for portability" ); #endif /* Return the first occurrence of NEEDLE in HAYSTACK. */ #if @GNULIB_MEMMEM@ # if @REPLACE_MEMMEM@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define memmem rpl_memmem # endif _GL_FUNCDECL_RPL (memmem, void *, (void const *__haystack, size_t __haystack_len, void const *__needle, size_t __needle_len) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 3))); _GL_CXXALIAS_RPL (memmem, void *, (void const *__haystack, size_t __haystack_len, void const *__needle, size_t __needle_len)); # else # if ! @HAVE_DECL_MEMMEM@ _GL_FUNCDECL_SYS (memmem, void *, (void const *__haystack, size_t __haystack_len, void const *__needle, size_t __needle_len) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 3))); # endif _GL_CXXALIAS_SYS (memmem, void *, (void const *__haystack, size_t __haystack_len, void const *__needle, size_t __needle_len)); # endif _GL_CXXALIASWARN (memmem); #elif defined GNULIB_POSIXCHECK # undef memmem # if HAVE_RAW_DECL_MEMMEM _GL_WARN_ON_USE (memmem, "memmem is unportable and often quadratic - " "use gnulib module memmem-simple for portability, " "and module memmem for speed" ); # endif #endif /* Copy N bytes of SRC to DEST, return pointer to bytes after the last written byte. */ #if @GNULIB_MEMPCPY@ # if ! @HAVE_MEMPCPY@ _GL_FUNCDECL_SYS (mempcpy, void *, (void *restrict __dest, void const *restrict __src, size_t __n) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (mempcpy, void *, (void *restrict __dest, void const *restrict __src, size_t __n)); _GL_CXXALIASWARN (mempcpy); #elif defined GNULIB_POSIXCHECK # undef mempcpy # if HAVE_RAW_DECL_MEMPCPY _GL_WARN_ON_USE (mempcpy, "mempcpy is unportable - " "use gnulib module mempcpy for portability"); # endif #endif /* Search backwards through a block for a byte (specified as an int). */ #if @GNULIB_MEMRCHR@ # if ! @HAVE_DECL_MEMRCHR@ _GL_FUNCDECL_SYS (memrchr, void *, (void const *, int, size_t) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const void * std::memrchr (const void *, int, size_t); } extern "C++" { void * std::memrchr (void *, int, size_t); } */ _GL_CXXALIAS_SYS_CAST2 (memrchr, void *, (void const *, int, size_t), void const *, (void const *, int, size_t)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (memrchr, void *, (void *, int, size_t)); _GL_CXXALIASWARN1 (memrchr, void const *, (void const *, int, size_t)); # else _GL_CXXALIASWARN (memrchr); # endif #elif defined GNULIB_POSIXCHECK # undef memrchr # if HAVE_RAW_DECL_MEMRCHR _GL_WARN_ON_USE (memrchr, "memrchr is unportable - " "use gnulib module memrchr for portability"); # endif #endif /* Find the first occurrence of C in S. More efficient than memchr(S,C,N), at the expense of undefined behavior if C does not occur within N bytes. */ #if @GNULIB_RAWMEMCHR@ # if ! @HAVE_RAWMEMCHR@ _GL_FUNCDECL_SYS (rawmemchr, void *, (void const *__s, int __c_in) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const void * std::rawmemchr (const void *, int); } extern "C++" { void * std::rawmemchr (void *, int); } */ _GL_CXXALIAS_SYS_CAST2 (rawmemchr, void *, (void const *__s, int __c_in), void const *, (void const *__s, int __c_in)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (rawmemchr, void *, (void *__s, int __c_in)); _GL_CXXALIASWARN1 (rawmemchr, void const *, (void const *__s, int __c_in)); # else _GL_CXXALIASWARN (rawmemchr); # endif #elif defined GNULIB_POSIXCHECK # undef rawmemchr # if HAVE_RAW_DECL_RAWMEMCHR _GL_WARN_ON_USE (rawmemchr, "rawmemchr is unportable - " "use gnulib module rawmemchr for portability"); # endif #endif /* Copy SRC to DST, returning the address of the terminating '\0' in DST. */ #if @GNULIB_STPCPY@ # if ! @HAVE_STPCPY@ _GL_FUNCDECL_SYS (stpcpy, char *, (char *restrict __dst, char const *restrict __src) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (stpcpy, char *, (char *restrict __dst, char const *restrict __src)); _GL_CXXALIASWARN (stpcpy); #elif defined GNULIB_POSIXCHECK # undef stpcpy # if HAVE_RAW_DECL_STPCPY _GL_WARN_ON_USE (stpcpy, "stpcpy is unportable - " "use gnulib module stpcpy for portability"); # endif #endif /* Copy no more than N bytes of SRC to DST, returning a pointer past the last non-NUL byte written into DST. */ #if @GNULIB_STPNCPY@ # if @REPLACE_STPNCPY@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef stpncpy # define stpncpy rpl_stpncpy # endif _GL_FUNCDECL_RPL (stpncpy, char *, (char *restrict __dst, char const *restrict __src, size_t __n) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (stpncpy, char *, (char *restrict __dst, char const *restrict __src, size_t __n)); # else # if ! @HAVE_STPNCPY@ _GL_FUNCDECL_SYS (stpncpy, char *, (char *restrict __dst, char const *restrict __src, size_t __n) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (stpncpy, char *, (char *restrict __dst, char const *restrict __src, size_t __n)); # endif _GL_CXXALIASWARN (stpncpy); #elif defined GNULIB_POSIXCHECK # undef stpncpy # if HAVE_RAW_DECL_STPNCPY _GL_WARN_ON_USE (stpncpy, "stpncpy is unportable - " "use gnulib module stpncpy for portability"); # endif #endif #if defined GNULIB_POSIXCHECK /* strchr() does not work with multibyte strings if the locale encoding is GB18030 and the character to be searched is a digit. */ # undef strchr /* Assume strchr is always declared. */ _GL_WARN_ON_USE (strchr, "strchr cannot work correctly on character strings " "in some multibyte locales - " "use mbschr if you care about internationalization"); #endif /* Find the first occurrence of C in S or the final NUL byte. */ #if @GNULIB_STRCHRNUL@ # if @REPLACE_STRCHRNUL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define strchrnul rpl_strchrnul # endif _GL_FUNCDECL_RPL (strchrnul, char *, (const char *__s, int __c_in) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (strchrnul, char *, (const char *str, int ch)); # else # if ! @HAVE_STRCHRNUL@ _GL_FUNCDECL_SYS (strchrnul, char *, (char const *__s, int __c_in) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const char * std::strchrnul (const char *, int); } extern "C++" { char * std::strchrnul (char *, int); } */ _GL_CXXALIAS_SYS_CAST2 (strchrnul, char *, (char const *__s, int __c_in), char const *, (char const *__s, int __c_in)); # endif # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (strchrnul, char *, (char *__s, int __c_in)); _GL_CXXALIASWARN1 (strchrnul, char const *, (char const *__s, int __c_in)); # else _GL_CXXALIASWARN (strchrnul); # endif #elif defined GNULIB_POSIXCHECK # undef strchrnul # if HAVE_RAW_DECL_STRCHRNUL _GL_WARN_ON_USE (strchrnul, "strchrnul is unportable - " "use gnulib module strchrnul for portability"); # endif #endif /* Duplicate S, returning an identical malloc'd string. */ #if @GNULIB_STRDUP@ # if @REPLACE_STRDUP@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strdup # define strdup rpl_strdup # endif _GL_FUNCDECL_RPL (strdup, char *, (char const *__s) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (strdup, char *, (char const *__s)); # else # if defined __cplusplus && defined GNULIB_NAMESPACE && defined strdup /* strdup exists as a function and as a macro. Get rid of the macro. */ # undef strdup # endif # if !(@HAVE_DECL_STRDUP@ || defined strdup) _GL_FUNCDECL_SYS (strdup, char *, (char const *__s) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strdup, char *, (char const *__s)); # endif _GL_CXXALIASWARN (strdup); #elif defined GNULIB_POSIXCHECK # undef strdup # if HAVE_RAW_DECL_STRDUP _GL_WARN_ON_USE (strdup, "strdup is unportable - " "use gnulib module strdup for portability"); # endif #endif /* Append no more than N characters from SRC onto DEST. */ #if @GNULIB_STRNCAT@ # if @REPLACE_STRNCAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strncat # define strncat rpl_strncat # endif _GL_FUNCDECL_RPL (strncat, char *, (char *dest, const char *src, size_t n) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (strncat, char *, (char *dest, const char *src, size_t n)); # else _GL_CXXALIAS_SYS (strncat, char *, (char *dest, const char *src, size_t n)); # endif _GL_CXXALIASWARN (strncat); #elif defined GNULIB_POSIXCHECK # undef strncat # if HAVE_RAW_DECL_STRNCAT _GL_WARN_ON_USE (strncat, "strncat is unportable - " "use gnulib module strncat for portability"); # endif #endif /* Return a newly allocated copy of at most N bytes of STRING. */ #if @GNULIB_STRNDUP@ # if @REPLACE_STRNDUP@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strndup # define strndup rpl_strndup # endif _GL_FUNCDECL_RPL (strndup, char *, (char const *__s, size_t __n) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (strndup, char *, (char const *__s, size_t __n)); # else # if ! @HAVE_DECL_STRNDUP@ _GL_FUNCDECL_SYS (strndup, char *, (char const *__s, size_t __n) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strndup, char *, (char const *__s, size_t __n)); # endif _GL_CXXALIASWARN (strndup); #elif defined GNULIB_POSIXCHECK # undef strndup # if HAVE_RAW_DECL_STRNDUP _GL_WARN_ON_USE (strndup, "strndup is unportable - " "use gnulib module strndup for portability"); # endif #endif /* Find the length (number of bytes) of STRING, but scan at most MAXLEN bytes. If no '\0' terminator is found in that many bytes, return MAXLEN. */ #if @GNULIB_STRNLEN@ # if @REPLACE_STRNLEN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strnlen # define strnlen rpl_strnlen # endif _GL_FUNCDECL_RPL (strnlen, size_t, (char const *__s, size_t __maxlen) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (strnlen, size_t, (char const *__s, size_t __maxlen)); # else # if ! @HAVE_DECL_STRNLEN@ _GL_FUNCDECL_SYS (strnlen, size_t, (char const *__s, size_t __maxlen) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strnlen, size_t, (char const *__s, size_t __maxlen)); # endif _GL_CXXALIASWARN (strnlen); #elif defined GNULIB_POSIXCHECK # undef strnlen # if HAVE_RAW_DECL_STRNLEN _GL_WARN_ON_USE (strnlen, "strnlen is unportable - " "use gnulib module strnlen for portability"); # endif #endif #if defined GNULIB_POSIXCHECK /* strcspn() assumes the second argument is a list of single-byte characters. Even in this simple case, it does not work with multibyte strings if the locale encoding is GB18030 and one of the characters to be searched is a digit. */ # undef strcspn /* Assume strcspn is always declared. */ _GL_WARN_ON_USE (strcspn, "strcspn cannot work correctly on character strings " "in multibyte locales - " "use mbscspn if you care about internationalization"); #endif /* Find the first occurrence in S of any character in ACCEPT. */ #if @GNULIB_STRPBRK@ # if ! @HAVE_STRPBRK@ _GL_FUNCDECL_SYS (strpbrk, char *, (char const *__s, char const *__accept) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2))); # endif /* On some systems, this function is defined as an overloaded function: extern "C" { const char * strpbrk (const char *, const char *); } extern "C++" { char * strpbrk (char *, const char *); } */ _GL_CXXALIAS_SYS_CAST2 (strpbrk, char *, (char const *__s, char const *__accept), const char *, (char const *__s, char const *__accept)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (strpbrk, char *, (char *__s, char const *__accept)); _GL_CXXALIASWARN1 (strpbrk, char const *, (char const *__s, char const *__accept)); # else _GL_CXXALIASWARN (strpbrk); # endif # if defined GNULIB_POSIXCHECK /* strpbrk() assumes the second argument is a list of single-byte characters. Even in this simple case, it does not work with multibyte strings if the locale encoding is GB18030 and one of the characters to be searched is a digit. */ # undef strpbrk _GL_WARN_ON_USE (strpbrk, "strpbrk cannot work correctly on character strings " "in multibyte locales - " "use mbspbrk if you care about internationalization"); # endif #elif defined GNULIB_POSIXCHECK # undef strpbrk # if HAVE_RAW_DECL_STRPBRK _GL_WARN_ON_USE (strpbrk, "strpbrk is unportable - " "use gnulib module strpbrk for portability"); # endif #endif #if defined GNULIB_POSIXCHECK /* strspn() assumes the second argument is a list of single-byte characters. Even in this simple case, it cannot work with multibyte strings. */ # undef strspn /* Assume strspn is always declared. */ _GL_WARN_ON_USE (strspn, "strspn cannot work correctly on character strings " "in multibyte locales - " "use mbsspn if you care about internationalization"); #endif #if defined GNULIB_POSIXCHECK /* strrchr() does not work with multibyte strings if the locale encoding is GB18030 and the character to be searched is a digit. */ # undef strrchr /* Assume strrchr is always declared. */ _GL_WARN_ON_USE (strrchr, "strrchr cannot work correctly on character strings " "in some multibyte locales - " "use mbsrchr if you care about internationalization"); #endif /* Search the next delimiter (char listed in DELIM) starting at *STRINGP. If one is found, overwrite it with a NUL, and advance *STRINGP to point to the next char after it. Otherwise, set *STRINGP to NULL. If *STRINGP was already NULL, nothing happens. Return the old value of *STRINGP. This is a variant of strtok() that is multithread-safe and supports empty fields. Caveat: It modifies the original string. Caveat: These functions cannot be used on constant strings. Caveat: The identity of the delimiting character is lost. Caveat: It doesn't work with multibyte strings unless all of the delimiter characters are ASCII characters < 0x30. See also strtok_r(). */ #if @GNULIB_STRSEP@ # if ! @HAVE_STRSEP@ _GL_FUNCDECL_SYS (strsep, char *, (char **restrict __stringp, char const *restrict __delim) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (strsep, char *, (char **restrict __stringp, char const *restrict __delim)); _GL_CXXALIASWARN (strsep); # if defined GNULIB_POSIXCHECK # undef strsep _GL_WARN_ON_USE (strsep, "strsep cannot work correctly on character strings " "in multibyte locales - " "use mbssep if you care about internationalization"); # endif #elif defined GNULIB_POSIXCHECK # undef strsep # if HAVE_RAW_DECL_STRSEP _GL_WARN_ON_USE (strsep, "strsep is unportable - " "use gnulib module strsep for portability"); # endif #endif #if @GNULIB_STRSTR@ # if @REPLACE_STRSTR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define strstr rpl_strstr # endif _GL_FUNCDECL_RPL (strstr, char *, (const char *haystack, const char *needle) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (strstr, char *, (const char *haystack, const char *needle)); # else /* On some systems, this function is defined as an overloaded function: extern "C++" { const char * strstr (const char *, const char *); } extern "C++" { char * strstr (char *, const char *); } */ _GL_CXXALIAS_SYS_CAST2 (strstr, char *, (const char *haystack, const char *needle), const char *, (const char *haystack, const char *needle)); # endif # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (strstr, char *, (char *haystack, const char *needle)); _GL_CXXALIASWARN1 (strstr, const char *, (const char *haystack, const char *needle)); # else _GL_CXXALIASWARN (strstr); # endif #elif defined GNULIB_POSIXCHECK /* strstr() does not work with multibyte strings if the locale encoding is different from UTF-8: POSIX says that it operates on "strings", and "string" in POSIX is defined as a sequence of bytes, not of characters. */ # undef strstr /* Assume strstr is always declared. */ _GL_WARN_ON_USE (strstr, "strstr is quadratic on many systems, and cannot " "work correctly on character strings in most " "multibyte locales - " "use mbsstr if you care about internationalization, " "or use strstr if you care about speed"); #endif /* Find the first occurrence of NEEDLE in HAYSTACK, using case-insensitive comparison. */ #if @GNULIB_STRCASESTR@ # if @REPLACE_STRCASESTR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define strcasestr rpl_strcasestr # endif _GL_FUNCDECL_RPL (strcasestr, char *, (const char *haystack, const char *needle) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (strcasestr, char *, (const char *haystack, const char *needle)); # else # if ! @HAVE_STRCASESTR@ _GL_FUNCDECL_SYS (strcasestr, char *, (const char *haystack, const char *needle) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2))); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const char * strcasestr (const char *, const char *); } extern "C++" { char * strcasestr (char *, const char *); } */ _GL_CXXALIAS_SYS_CAST2 (strcasestr, char *, (const char *haystack, const char *needle), const char *, (const char *haystack, const char *needle)); # endif # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (strcasestr, char *, (char *haystack, const char *needle)); _GL_CXXALIASWARN1 (strcasestr, const char *, (const char *haystack, const char *needle)); # else _GL_CXXALIASWARN (strcasestr); # endif #elif defined GNULIB_POSIXCHECK /* strcasestr() does not work with multibyte strings: It is a glibc extension, and glibc implements it only for unibyte locales. */ # undef strcasestr # if HAVE_RAW_DECL_STRCASESTR _GL_WARN_ON_USE (strcasestr, "strcasestr does work correctly on character " "strings in multibyte locales - " "use mbscasestr if you care about " "internationalization, or use c-strcasestr if you want " "a locale independent function"); # endif #endif /* Parse S into tokens separated by characters in DELIM. If S is NULL, the saved pointer in SAVE_PTR is used as the next starting point. For example: char s[] = "-abc-=-def"; char *sp; x = strtok_r(s, "-", &sp); // x = "abc", sp = "=-def" x = strtok_r(NULL, "-=", &sp); // x = "def", sp = NULL x = strtok_r(NULL, "=", &sp); // x = NULL // s = "abc\0-def\0" This is a variant of strtok() that is multithread-safe. For the POSIX documentation for this function, see: http://www.opengroup.org/susv3xsh/strtok.html Caveat: It modifies the original string. Caveat: These functions cannot be used on constant strings. Caveat: The identity of the delimiting character is lost. Caveat: It doesn't work with multibyte strings unless all of the delimiter characters are ASCII characters < 0x30. See also strsep(). */ #if @GNULIB_STRTOK_R@ # if @REPLACE_STRTOK_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strtok_r # define strtok_r rpl_strtok_r # endif _GL_FUNCDECL_RPL (strtok_r, char *, (char *restrict s, char const *restrict delim, char **restrict save_ptr) _GL_ARG_NONNULL ((2, 3))); _GL_CXXALIAS_RPL (strtok_r, char *, (char *restrict s, char const *restrict delim, char **restrict save_ptr)); # else # if @UNDEFINE_STRTOK_R@ || defined GNULIB_POSIXCHECK # undef strtok_r # endif # if ! @HAVE_DECL_STRTOK_R@ _GL_FUNCDECL_SYS (strtok_r, char *, (char *restrict s, char const *restrict delim, char **restrict save_ptr) _GL_ARG_NONNULL ((2, 3))); # endif _GL_CXXALIAS_SYS (strtok_r, char *, (char *restrict s, char const *restrict delim, char **restrict save_ptr)); # endif _GL_CXXALIASWARN (strtok_r); # if defined GNULIB_POSIXCHECK _GL_WARN_ON_USE (strtok_r, "strtok_r cannot work correctly on character " "strings in multibyte locales - " "use mbstok_r if you care about internationalization"); # endif #elif defined GNULIB_POSIXCHECK # undef strtok_r # if HAVE_RAW_DECL_STRTOK_R _GL_WARN_ON_USE (strtok_r, "strtok_r is unportable - " "use gnulib module strtok_r for portability"); # endif #endif /* The following functions are not specified by POSIX. They are gnulib extensions. */ #if @GNULIB_MBSLEN@ /* Return the number of multibyte characters in the character string STRING. This considers multibyte characters, unlike strlen, which counts bytes. */ # ifdef __MirBSD__ /* MirBSD defines mbslen as a macro. Override it. */ # undef mbslen # endif # if @HAVE_MBSLEN@ /* AIX, OSF/1, MirBSD define mbslen already in libc. */ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define mbslen rpl_mbslen # endif _GL_FUNCDECL_RPL (mbslen, size_t, (const char *string) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mbslen, size_t, (const char *string)); # else _GL_FUNCDECL_SYS (mbslen, size_t, (const char *string) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_SYS (mbslen, size_t, (const char *string)); # endif _GL_CXXALIASWARN (mbslen); #endif #if @GNULIB_MBSNLEN@ /* Return the number of multibyte characters in the character string starting at STRING and ending at STRING + LEN. */ _GL_EXTERN_C size_t mbsnlen (const char *string, size_t len) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1)); #endif #if @GNULIB_MBSCHR@ /* Locate the first single-byte character C in the character string STRING, and return a pointer to it. Return NULL if C is not found in STRING. Unlike strchr(), this function works correctly in multibyte locales with encodings such as GB18030. */ # if defined __hpux # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define mbschr rpl_mbschr /* avoid collision with HP-UX function */ # endif _GL_FUNCDECL_RPL (mbschr, char *, (const char *string, int c) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mbschr, char *, (const char *string, int c)); # else _GL_FUNCDECL_SYS (mbschr, char *, (const char *string, int c) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_SYS (mbschr, char *, (const char *string, int c)); # endif _GL_CXXALIASWARN (mbschr); #endif #if @GNULIB_MBSRCHR@ /* Locate the last single-byte character C in the character string STRING, and return a pointer to it. Return NULL if C is not found in STRING. Unlike strrchr(), this function works correctly in multibyte locales with encodings such as GB18030. */ # if defined __hpux || defined __INTERIX # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define mbsrchr rpl_mbsrchr /* avoid collision with system function */ # endif _GL_FUNCDECL_RPL (mbsrchr, char *, (const char *string, int c) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mbsrchr, char *, (const char *string, int c)); # else _GL_FUNCDECL_SYS (mbsrchr, char *, (const char *string, int c) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_SYS (mbsrchr, char *, (const char *string, int c)); # endif _GL_CXXALIASWARN (mbsrchr); #endif #if @GNULIB_MBSSTR@ /* Find the first occurrence of the character string NEEDLE in the character string HAYSTACK. Return NULL if NEEDLE is not found in HAYSTACK. Unlike strstr(), this function works correctly in multibyte locales with encodings different from UTF-8. */ _GL_EXTERN_C char * mbsstr (const char *haystack, const char *needle) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSCASECMP@ /* Compare the character strings S1 and S2, ignoring case, returning less than, equal to or greater than zero if S1 is lexicographically less than, equal to or greater than S2. Note: This function may, in multibyte locales, return 0 for strings of different lengths! Unlike strcasecmp(), this function works correctly in multibyte locales. */ _GL_EXTERN_C int mbscasecmp (const char *s1, const char *s2) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSNCASECMP@ /* Compare the initial segment of the character string S1 consisting of at most N characters with the initial segment of the character string S2 consisting of at most N characters, ignoring case, returning less than, equal to or greater than zero if the initial segment of S1 is lexicographically less than, equal to or greater than the initial segment of S2. Note: This function may, in multibyte locales, return 0 for initial segments of different lengths! Unlike strncasecmp(), this function works correctly in multibyte locales. But beware that N is not a byte count but a character count! */ _GL_EXTERN_C int mbsncasecmp (const char *s1, const char *s2, size_t n) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSPCASECMP@ /* Compare the initial segment of the character string STRING consisting of at most mbslen (PREFIX) characters with the character string PREFIX, ignoring case. If the two match, return a pointer to the first byte after this prefix in STRING. Otherwise, return NULL. Note: This function may, in multibyte locales, return non-NULL if STRING is of smaller length than PREFIX! Unlike strncasecmp(), this function works correctly in multibyte locales. */ _GL_EXTERN_C char * mbspcasecmp (const char *string, const char *prefix) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSCASESTR@ /* Find the first occurrence of the character string NEEDLE in the character string HAYSTACK, using case-insensitive comparison. Note: This function may, in multibyte locales, return success even if strlen (haystack) < strlen (needle) ! Unlike strcasestr(), this function works correctly in multibyte locales. */ _GL_EXTERN_C char * mbscasestr (const char *haystack, const char *needle) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSCSPN@ /* Find the first occurrence in the character string STRING of any character in the character string ACCEPT. Return the number of bytes from the beginning of the string to this occurrence, or to the end of the string if none exists. Unlike strcspn(), this function works correctly in multibyte locales. */ _GL_EXTERN_C size_t mbscspn (const char *string, const char *accept) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSPBRK@ /* Find the first occurrence in the character string STRING of any character in the character string ACCEPT. Return the pointer to it, or NULL if none exists. Unlike strpbrk(), this function works correctly in multibyte locales. */ # if defined __hpux # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define mbspbrk rpl_mbspbrk /* avoid collision with HP-UX function */ # endif _GL_FUNCDECL_RPL (mbspbrk, char *, (const char *string, const char *accept) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (mbspbrk, char *, (const char *string, const char *accept)); # else _GL_FUNCDECL_SYS (mbspbrk, char *, (const char *string, const char *accept) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_SYS (mbspbrk, char *, (const char *string, const char *accept)); # endif _GL_CXXALIASWARN (mbspbrk); #endif #if @GNULIB_MBSSPN@ /* Find the first occurrence in the character string STRING of any character not in the character string REJECT. Return the number of bytes from the beginning of the string to this occurrence, or to the end of the string if none exists. Unlike strspn(), this function works correctly in multibyte locales. */ _GL_EXTERN_C size_t mbsspn (const char *string, const char *reject) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSSEP@ /* Search the next delimiter (multibyte character listed in the character string DELIM) starting at the character string *STRINGP. If one is found, overwrite it with a NUL, and advance *STRINGP to point to the next multibyte character after it. Otherwise, set *STRINGP to NULL. If *STRINGP was already NULL, nothing happens. Return the old value of *STRINGP. This is a variant of mbstok_r() that supports empty fields. Caveat: It modifies the original string. Caveat: These functions cannot be used on constant strings. Caveat: The identity of the delimiting character is lost. See also mbstok_r(). */ _GL_EXTERN_C char * mbssep (char **stringp, const char *delim) _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSTOK_R@ /* Parse the character string STRING into tokens separated by characters in the character string DELIM. If STRING is NULL, the saved pointer in SAVE_PTR is used as the next starting point. For example: char s[] = "-abc-=-def"; char *sp; x = mbstok_r(s, "-", &sp); // x = "abc", sp = "=-def" x = mbstok_r(NULL, "-=", &sp); // x = "def", sp = NULL x = mbstok_r(NULL, "=", &sp); // x = NULL // s = "abc\0-def\0" Caveat: It modifies the original string. Caveat: These functions cannot be used on constant strings. Caveat: The identity of the delimiting character is lost. See also mbssep(). */ _GL_EXTERN_C char * mbstok_r (char *string, const char *delim, char **save_ptr) _GL_ARG_NONNULL ((2, 3)); #endif /* Map any int, typically from errno, into an error message. */ #if @GNULIB_STRERROR@ # if @REPLACE_STRERROR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strerror # define strerror rpl_strerror # endif _GL_FUNCDECL_RPL (strerror, char *, (int)); _GL_CXXALIAS_RPL (strerror, char *, (int)); # else _GL_CXXALIAS_SYS (strerror, char *, (int)); # endif _GL_CXXALIASWARN (strerror); #elif defined GNULIB_POSIXCHECK # undef strerror /* Assume strerror is always declared. */ _GL_WARN_ON_USE (strerror, "strerror is unportable - " "use gnulib module strerror to guarantee non-NULL result"); #endif /* Map any int, typically from errno, into an error message. Multithread-safe. Uses the POSIX declaration, not the glibc declaration. */ #if @GNULIB_STRERROR_R@ # if @REPLACE_STRERROR_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strerror_r # define strerror_r rpl_strerror_r # endif _GL_FUNCDECL_RPL (strerror_r, int, (int errnum, char *buf, size_t buflen) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (strerror_r, int, (int errnum, char *buf, size_t buflen)); # else # if !@HAVE_DECL_STRERROR_R@ _GL_FUNCDECL_SYS (strerror_r, int, (int errnum, char *buf, size_t buflen) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (strerror_r, int, (int errnum, char *buf, size_t buflen)); # endif # if @HAVE_DECL_STRERROR_R@ _GL_CXXALIASWARN (strerror_r); # endif #elif defined GNULIB_POSIXCHECK # undef strerror_r # if HAVE_RAW_DECL_STRERROR_R _GL_WARN_ON_USE (strerror_r, "strerror_r is unportable - " "use gnulib module strerror_r-posix for portability"); # endif #endif #if @GNULIB_STRSIGNAL@ # if @REPLACE_STRSIGNAL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define strsignal rpl_strsignal # endif _GL_FUNCDECL_RPL (strsignal, char *, (int __sig)); _GL_CXXALIAS_RPL (strsignal, char *, (int __sig)); # else # if ! @HAVE_DECL_STRSIGNAL@ _GL_FUNCDECL_SYS (strsignal, char *, (int __sig)); # endif /* Need to cast, because on Cygwin 1.5.x systems, the return type is 'const char *'. */ _GL_CXXALIAS_SYS_CAST (strsignal, char *, (int __sig)); # endif _GL_CXXALIASWARN (strsignal); #elif defined GNULIB_POSIXCHECK # undef strsignal # if HAVE_RAW_DECL_STRSIGNAL _GL_WARN_ON_USE (strsignal, "strsignal is unportable - " "use gnulib module strsignal for portability"); # endif #endif #if @GNULIB_STRVERSCMP@ # if !@HAVE_STRVERSCMP@ _GL_FUNCDECL_SYS (strverscmp, int, (const char *, const char *) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (strverscmp, int, (const char *, const char *)); _GL_CXXALIASWARN (strverscmp); #elif defined GNULIB_POSIXCHECK # undef strverscmp # if HAVE_RAW_DECL_STRVERSCMP _GL_WARN_ON_USE (strverscmp, "strverscmp is unportable - " "use gnulib module strverscmp for portability"); # endif #endif #endif /* _@GUARD_PREFIX@_STRING_H */ #endif /* _@GUARD_PREFIX@_STRING_H */ #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/strerror-override.h0000644000175000017500000000374313004436754020256 00000000000000/* strerror-override.h --- POSIX compatible system error routine Copyright (C) 2010-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _GL_STRERROR_OVERRIDE_H # define _GL_STRERROR_OVERRIDE_H # include # include /* Reasonable buffer size that should never trigger ERANGE; if this proves too small, we intentionally abort(), to remind us to fix this value. */ # define STACKBUF_LEN 256 /* If ERRNUM maps to an errno value defined by gnulib, return a string describing the error. Otherwise return NULL. */ # if REPLACE_STRERROR_0 \ || GNULIB_defined_ESOCK \ || GNULIB_defined_ESTREAMS \ || GNULIB_defined_EWINSOCK \ || GNULIB_defined_ENOMSG \ || GNULIB_defined_EIDRM \ || GNULIB_defined_ENOLINK \ || GNULIB_defined_EPROTO \ || GNULIB_defined_EMULTIHOP \ || GNULIB_defined_EBADMSG \ || GNULIB_defined_EOVERFLOW \ || GNULIB_defined_ENOTSUP \ || GNULIB_defined_ENETRESET \ || GNULIB_defined_ECONNABORTED \ || GNULIB_defined_ESTALE \ || GNULIB_defined_EDQUOT \ || GNULIB_defined_ECANCELED \ || GNULIB_defined_EOWNERDEAD \ || GNULIB_defined_ENOTRECOVERABLE \ || GNULIB_defined_EILSEQ extern const char *strerror_override (int errnum) _GL_ATTRIBUTE_CONST; # else # define strerror_override(ignored) NULL # endif #endif /* _GL_STRERROR_OVERRIDE_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/streq.h0000644000175000017500000000763613004436754015722 00000000000000/* Optimized string comparison. Copyright (C) 2001-2002, 2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible . */ #ifndef _GL_STREQ_H #define _GL_STREQ_H #include /* STREQ_OPT allows to optimize string comparison with a small literal string. STREQ_OPT (s, "EUC-KR", 'E', 'U', 'C', '-', 'K', 'R', 0, 0, 0) is semantically equivalent to strcmp (s, "EUC-KR") == 0 just faster. */ /* Help GCC to generate good code for string comparisons with immediate strings. */ #if defined (__GNUC__) && defined (__OPTIMIZE__) static inline int streq9 (const char *s1, const char *s2) { return strcmp (s1 + 9, s2 + 9) == 0; } static inline int streq8 (const char *s1, const char *s2, char s28) { if (s1[8] == s28) { if (s28 == 0) return 1; else return streq9 (s1, s2); } else return 0; } static inline int streq7 (const char *s1, const char *s2, char s27, char s28) { if (s1[7] == s27) { if (s27 == 0) return 1; else return streq8 (s1, s2, s28); } else return 0; } static inline int streq6 (const char *s1, const char *s2, char s26, char s27, char s28) { if (s1[6] == s26) { if (s26 == 0) return 1; else return streq7 (s1, s2, s27, s28); } else return 0; } static inline int streq5 (const char *s1, const char *s2, char s25, char s26, char s27, char s28) { if (s1[5] == s25) { if (s25 == 0) return 1; else return streq6 (s1, s2, s26, s27, s28); } else return 0; } static inline int streq4 (const char *s1, const char *s2, char s24, char s25, char s26, char s27, char s28) { if (s1[4] == s24) { if (s24 == 0) return 1; else return streq5 (s1, s2, s25, s26, s27, s28); } else return 0; } static inline int streq3 (const char *s1, const char *s2, char s23, char s24, char s25, char s26, char s27, char s28) { if (s1[3] == s23) { if (s23 == 0) return 1; else return streq4 (s1, s2, s24, s25, s26, s27, s28); } else return 0; } static inline int streq2 (const char *s1, const char *s2, char s22, char s23, char s24, char s25, char s26, char s27, char s28) { if (s1[2] == s22) { if (s22 == 0) return 1; else return streq3 (s1, s2, s23, s24, s25, s26, s27, s28); } else return 0; } static inline int streq1 (const char *s1, const char *s2, char s21, char s22, char s23, char s24, char s25, char s26, char s27, char s28) { if (s1[1] == s21) { if (s21 == 0) return 1; else return streq2 (s1, s2, s22, s23, s24, s25, s26, s27, s28); } else return 0; } static inline int streq0 (const char *s1, const char *s2, char s20, char s21, char s22, char s23, char s24, char s25, char s26, char s27, char s28) { if (s1[0] == s20) { if (s20 == 0) return 1; else return streq1 (s1, s2, s21, s22, s23, s24, s25, s26, s27, s28); } else return 0; } #define STREQ_OPT(s1,s2,s20,s21,s22,s23,s24,s25,s26,s27,s28) \ streq0 (s1, s2, s20, s21, s22, s23, s24, s25, s26, s27, s28) #else #define STREQ_OPT(s1,s2,s20,s21,s22,s23,s24,s25,s26,s27,s28) \ (strcmp (s1, s2) == 0) #endif #endif /* _GL_STREQ_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/strchrnul.valgrind0000644000175000017500000000040313004436754020150 00000000000000# Suppress a valgrind message about use of uninitialized memory in strchrnul(). # This use is OK because it provides only a speedup. { strchrnul-value4 Memcheck:Value4 fun:strchrnul } { strchrnul-value8 Memcheck:Value8 fun:strchrnul } gnuastro-0.2.33-8a3b/bootstrapped/lib/stdlib.in.h0000644000175000017500000010371213004436754016442 00000000000000/* A GNU-like . Copyright (C) 1995, 2001-2004, 2006-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if defined __need_system_stdlib_h || defined __need_malloc_and_calloc /* Special invocation conventions inside some gnulib header files, and inside some glibc header files, respectively. */ #@INCLUDE_NEXT@ @NEXT_STDLIB_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_STDLIB_H /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_STDLIB_H@ #ifndef _@GUARD_PREFIX@_STDLIB_H #define _@GUARD_PREFIX@_STDLIB_H /* NetBSD 5.0 mis-defines NULL. */ #include /* MirBSD 10 defines WEXITSTATUS in , not in . */ #if @GNULIB_SYSTEM_POSIX@ && !defined WEXITSTATUS # include #endif /* Solaris declares getloadavg() in . */ #if (@GNULIB_GETLOADAVG@ || defined GNULIB_POSIXCHECK) && @HAVE_SYS_LOADAVG_H@ # include #endif /* Native Windows platforms declare mktemp() in . */ #if 0 && ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) # include #endif #if @GNULIB_RANDOM_R@ /* OSF/1 5.1 declares 'struct random_data' in , which is included from if _REENTRANT is defined. Include it whenever we need 'struct random_data'. */ # if @HAVE_RANDOM_H@ # include # endif # if !@HAVE_STRUCT_RANDOM_DATA@ || @REPLACE_RANDOM_R@ || !@HAVE_RANDOM_R@ # include # endif # if !@HAVE_STRUCT_RANDOM_DATA@ /* Define 'struct random_data'. But allow multiple gnulib generated replacements to coexist. */ # if !GNULIB_defined_struct_random_data struct random_data { int32_t *fptr; /* Front pointer. */ int32_t *rptr; /* Rear pointer. */ int32_t *state; /* Array of state values. */ int rand_type; /* Type of random number generator. */ int rand_deg; /* Degree of random number generator. */ int rand_sep; /* Distance between front and rear. */ int32_t *end_ptr; /* Pointer behind state table. */ }; # define GNULIB_defined_struct_random_data 1 # endif # endif #endif #if (@GNULIB_MKSTEMP@ || @GNULIB_MKSTEMPS@ || @GNULIB_GETSUBOPT@ || defined GNULIB_POSIXCHECK) && ! defined __GLIBC__ && !((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) /* On Mac OS X 10.3, only declares mkstemp. */ /* On Mac OS X 10.5, only declares mkstemps. */ /* On Cygwin 1.7.1, only declares getsubopt. */ /* But avoid namespace pollution on glibc systems and native Windows. */ # include #endif /* The __attribute__ feature is available in gcc versions 2.5 and later. The attribute __pure__ was added in gcc 2.96. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 96) # define _GL_ATTRIBUTE_PURE __attribute__ ((__pure__)) #else # define _GL_ATTRIBUTE_PURE /* empty */ #endif /* The definition of _Noreturn is copied here. */ /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Some systems do not define EXIT_*, despite otherwise supporting C89. */ #ifndef EXIT_SUCCESS # define EXIT_SUCCESS 0 #endif /* Tandem/NSK and other platforms that define EXIT_FAILURE as -1 interfere with proper operation of xargs. */ #ifndef EXIT_FAILURE # define EXIT_FAILURE 1 #elif EXIT_FAILURE != 1 # undef EXIT_FAILURE # define EXIT_FAILURE 1 #endif #if @GNULIB__EXIT@ /* Terminate the current process with the given return code, without running the 'atexit' handlers. */ # if !@HAVE__EXIT@ _GL_FUNCDECL_SYS (_Exit, _Noreturn void, (int status)); # endif _GL_CXXALIAS_SYS (_Exit, void, (int status)); _GL_CXXALIASWARN (_Exit); #elif defined GNULIB_POSIXCHECK # undef _Exit # if HAVE_RAW_DECL__EXIT _GL_WARN_ON_USE (_Exit, "_Exit is unportable - " "use gnulib module _Exit for portability"); # endif #endif #if @GNULIB_ATOLL@ /* Parse a signed decimal integer. Returns the value of the integer. Errors are not detected. */ # if !@HAVE_ATOLL@ _GL_FUNCDECL_SYS (atoll, long long, (const char *string) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (atoll, long long, (const char *string)); _GL_CXXALIASWARN (atoll); #elif defined GNULIB_POSIXCHECK # undef atoll # if HAVE_RAW_DECL_ATOLL _GL_WARN_ON_USE (atoll, "atoll is unportable - " "use gnulib module atoll for portability"); # endif #endif #if @GNULIB_CALLOC_POSIX@ # if @REPLACE_CALLOC@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef calloc # define calloc rpl_calloc # endif _GL_FUNCDECL_RPL (calloc, void *, (size_t nmemb, size_t size)); _GL_CXXALIAS_RPL (calloc, void *, (size_t nmemb, size_t size)); # else _GL_CXXALIAS_SYS (calloc, void *, (size_t nmemb, size_t size)); # endif _GL_CXXALIASWARN (calloc); #elif defined GNULIB_POSIXCHECK # undef calloc /* Assume calloc is always declared. */ _GL_WARN_ON_USE (calloc, "calloc is not POSIX compliant everywhere - " "use gnulib module calloc-posix for portability"); #endif #if @GNULIB_CANONICALIZE_FILE_NAME@ # if @REPLACE_CANONICALIZE_FILE_NAME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define canonicalize_file_name rpl_canonicalize_file_name # endif _GL_FUNCDECL_RPL (canonicalize_file_name, char *, (const char *name) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (canonicalize_file_name, char *, (const char *name)); # else # if !@HAVE_CANONICALIZE_FILE_NAME@ _GL_FUNCDECL_SYS (canonicalize_file_name, char *, (const char *name) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (canonicalize_file_name, char *, (const char *name)); # endif _GL_CXXALIASWARN (canonicalize_file_name); #elif defined GNULIB_POSIXCHECK # undef canonicalize_file_name # if HAVE_RAW_DECL_CANONICALIZE_FILE_NAME _GL_WARN_ON_USE (canonicalize_file_name, "canonicalize_file_name is unportable - " "use gnulib module canonicalize-lgpl for portability"); # endif #endif #if @GNULIB_GETLOADAVG@ /* Store max(NELEM,3) load average numbers in LOADAVG[]. The three numbers are the load average of the last 1 minute, the last 5 minutes, and the last 15 minutes, respectively. LOADAVG is an array of NELEM numbers. */ # if !@HAVE_DECL_GETLOADAVG@ _GL_FUNCDECL_SYS (getloadavg, int, (double loadavg[], int nelem) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (getloadavg, int, (double loadavg[], int nelem)); _GL_CXXALIASWARN (getloadavg); #elif defined GNULIB_POSIXCHECK # undef getloadavg # if HAVE_RAW_DECL_GETLOADAVG _GL_WARN_ON_USE (getloadavg, "getloadavg is not portable - " "use gnulib module getloadavg for portability"); # endif #endif #if @GNULIB_GETSUBOPT@ /* Assuming *OPTIONP is a comma separated list of elements of the form "token" or "token=value", getsubopt parses the first of these elements. If the first element refers to a "token" that is member of the given NULL-terminated array of tokens: - It replaces the comma with a NUL byte, updates *OPTIONP to point past the first option and the comma, sets *VALUEP to the value of the element (or NULL if it doesn't contain an "=" sign), - It returns the index of the "token" in the given array of tokens. Otherwise it returns -1, and *OPTIONP and *VALUEP are undefined. For more details see the POSIX:2001 specification. http://www.opengroup.org/susv3xsh/getsubopt.html */ # if !@HAVE_GETSUBOPT@ _GL_FUNCDECL_SYS (getsubopt, int, (char **optionp, char *const *tokens, char **valuep) _GL_ARG_NONNULL ((1, 2, 3))); # endif _GL_CXXALIAS_SYS (getsubopt, int, (char **optionp, char *const *tokens, char **valuep)); _GL_CXXALIASWARN (getsubopt); #elif defined GNULIB_POSIXCHECK # undef getsubopt # if HAVE_RAW_DECL_GETSUBOPT _GL_WARN_ON_USE (getsubopt, "getsubopt is unportable - " "use gnulib module getsubopt for portability"); # endif #endif #if @GNULIB_GRANTPT@ /* Change the ownership and access permission of the slave side of the pseudo-terminal whose master side is specified by FD. */ # if !@HAVE_GRANTPT@ _GL_FUNCDECL_SYS (grantpt, int, (int fd)); # endif _GL_CXXALIAS_SYS (grantpt, int, (int fd)); _GL_CXXALIASWARN (grantpt); #elif defined GNULIB_POSIXCHECK # undef grantpt # if HAVE_RAW_DECL_GRANTPT _GL_WARN_ON_USE (grantpt, "grantpt is not portable - " "use gnulib module grantpt for portability"); # endif #endif /* If _GL_USE_STDLIB_ALLOC is nonzero, the including module does not rely on GNU or POSIX semantics for malloc and realloc (for example, by never specifying a zero size), so it does not need malloc or realloc to be redefined. */ #if @GNULIB_MALLOC_POSIX@ # if @REPLACE_MALLOC@ # if !((defined __cplusplus && defined GNULIB_NAMESPACE) \ || _GL_USE_STDLIB_ALLOC) # undef malloc # define malloc rpl_malloc # endif _GL_FUNCDECL_RPL (malloc, void *, (size_t size)); _GL_CXXALIAS_RPL (malloc, void *, (size_t size)); # else _GL_CXXALIAS_SYS (malloc, void *, (size_t size)); # endif _GL_CXXALIASWARN (malloc); #elif defined GNULIB_POSIXCHECK && !_GL_USE_STDLIB_ALLOC # undef malloc /* Assume malloc is always declared. */ _GL_WARN_ON_USE (malloc, "malloc is not POSIX compliant everywhere - " "use gnulib module malloc-posix for portability"); #endif /* Convert a multibyte character to a wide character. */ #if @GNULIB_MBTOWC@ # if @REPLACE_MBTOWC@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mbtowc # define mbtowc rpl_mbtowc # endif _GL_FUNCDECL_RPL (mbtowc, int, (wchar_t *pwc, const char *s, size_t n)); _GL_CXXALIAS_RPL (mbtowc, int, (wchar_t *pwc, const char *s, size_t n)); # else _GL_CXXALIAS_SYS (mbtowc, int, (wchar_t *pwc, const char *s, size_t n)); # endif _GL_CXXALIASWARN (mbtowc); #endif #if @GNULIB_MKDTEMP@ /* Create a unique temporary directory from TEMPLATE. The last six characters of TEMPLATE must be "XXXXXX"; they are replaced with a string that makes the directory name unique. Returns TEMPLATE, or a null pointer if it cannot get a unique name. The directory is created mode 700. */ # if !@HAVE_MKDTEMP@ _GL_FUNCDECL_SYS (mkdtemp, char *, (char * /*template*/) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (mkdtemp, char *, (char * /*template*/)); _GL_CXXALIASWARN (mkdtemp); #elif defined GNULIB_POSIXCHECK # undef mkdtemp # if HAVE_RAW_DECL_MKDTEMP _GL_WARN_ON_USE (mkdtemp, "mkdtemp is unportable - " "use gnulib module mkdtemp for portability"); # endif #endif #if @GNULIB_MKOSTEMP@ /* Create a unique temporary file from TEMPLATE. The last six characters of TEMPLATE must be "XXXXXX"; they are replaced with a string that makes the file name unique. The flags are a bitmask, possibly including O_CLOEXEC (defined in ) and O_TEXT, O_BINARY (defined in "binary-io.h"). The file is then created, with the specified flags, ensuring it didn't exist before. The file is created read-write (mask at least 0600 & ~umask), but it may be world-readable and world-writable (mask 0666 & ~umask), depending on the implementation. Returns the open file descriptor if successful, otherwise -1 and errno set. */ # if !@HAVE_MKOSTEMP@ _GL_FUNCDECL_SYS (mkostemp, int, (char * /*template*/, int /*flags*/) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (mkostemp, int, (char * /*template*/, int /*flags*/)); _GL_CXXALIASWARN (mkostemp); #elif defined GNULIB_POSIXCHECK # undef mkostemp # if HAVE_RAW_DECL_MKOSTEMP _GL_WARN_ON_USE (mkostemp, "mkostemp is unportable - " "use gnulib module mkostemp for portability"); # endif #endif #if @GNULIB_MKOSTEMPS@ /* Create a unique temporary file from TEMPLATE. The last six characters of TEMPLATE before a suffix of length SUFFIXLEN must be "XXXXXX"; they are replaced with a string that makes the file name unique. The flags are a bitmask, possibly including O_CLOEXEC (defined in ) and O_TEXT, O_BINARY (defined in "binary-io.h"). The file is then created, with the specified flags, ensuring it didn't exist before. The file is created read-write (mask at least 0600 & ~umask), but it may be world-readable and world-writable (mask 0666 & ~umask), depending on the implementation. Returns the open file descriptor if successful, otherwise -1 and errno set. */ # if !@HAVE_MKOSTEMPS@ _GL_FUNCDECL_SYS (mkostemps, int, (char * /*template*/, int /*suffixlen*/, int /*flags*/) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (mkostemps, int, (char * /*template*/, int /*suffixlen*/, int /*flags*/)); _GL_CXXALIASWARN (mkostemps); #elif defined GNULIB_POSIXCHECK # undef mkostemps # if HAVE_RAW_DECL_MKOSTEMPS _GL_WARN_ON_USE (mkostemps, "mkostemps is unportable - " "use gnulib module mkostemps for portability"); # endif #endif #if @GNULIB_MKSTEMP@ /* Create a unique temporary file from TEMPLATE. The last six characters of TEMPLATE must be "XXXXXX"; they are replaced with a string that makes the file name unique. The file is then created, ensuring it didn't exist before. The file is created read-write (mask at least 0600 & ~umask), but it may be world-readable and world-writable (mask 0666 & ~umask), depending on the implementation. Returns the open file descriptor if successful, otherwise -1 and errno set. */ # if @REPLACE_MKSTEMP@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define mkstemp rpl_mkstemp # endif _GL_FUNCDECL_RPL (mkstemp, int, (char * /*template*/) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mkstemp, int, (char * /*template*/)); # else # if ! @HAVE_MKSTEMP@ _GL_FUNCDECL_SYS (mkstemp, int, (char * /*template*/) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (mkstemp, int, (char * /*template*/)); # endif _GL_CXXALIASWARN (mkstemp); #elif defined GNULIB_POSIXCHECK # undef mkstemp # if HAVE_RAW_DECL_MKSTEMP _GL_WARN_ON_USE (mkstemp, "mkstemp is unportable - " "use gnulib module mkstemp for portability"); # endif #endif #if @GNULIB_MKSTEMPS@ /* Create a unique temporary file from TEMPLATE. The last six characters of TEMPLATE prior to a suffix of length SUFFIXLEN must be "XXXXXX"; they are replaced with a string that makes the file name unique. The file is then created, ensuring it didn't exist before. The file is created read-write (mask at least 0600 & ~umask), but it may be world-readable and world-writable (mask 0666 & ~umask), depending on the implementation. Returns the open file descriptor if successful, otherwise -1 and errno set. */ # if !@HAVE_MKSTEMPS@ _GL_FUNCDECL_SYS (mkstemps, int, (char * /*template*/, int /*suffixlen*/) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (mkstemps, int, (char * /*template*/, int /*suffixlen*/)); _GL_CXXALIASWARN (mkstemps); #elif defined GNULIB_POSIXCHECK # undef mkstemps # if HAVE_RAW_DECL_MKSTEMPS _GL_WARN_ON_USE (mkstemps, "mkstemps is unportable - " "use gnulib module mkstemps for portability"); # endif #endif #if @GNULIB_POSIX_OPENPT@ /* Return an FD open to the master side of a pseudo-terminal. Flags should include O_RDWR, and may also include O_NOCTTY. */ # if !@HAVE_POSIX_OPENPT@ _GL_FUNCDECL_SYS (posix_openpt, int, (int flags)); # endif _GL_CXXALIAS_SYS (posix_openpt, int, (int flags)); _GL_CXXALIASWARN (posix_openpt); #elif defined GNULIB_POSIXCHECK # undef posix_openpt # if HAVE_RAW_DECL_POSIX_OPENPT _GL_WARN_ON_USE (posix_openpt, "posix_openpt is not portable - " "use gnulib module posix_openpt for portability"); # endif #endif #if @GNULIB_PTSNAME@ /* Return the pathname of the pseudo-terminal slave associated with the master FD is open on, or NULL on errors. */ # if @REPLACE_PTSNAME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ptsname # define ptsname rpl_ptsname # endif _GL_FUNCDECL_RPL (ptsname, char *, (int fd)); _GL_CXXALIAS_RPL (ptsname, char *, (int fd)); # else # if !@HAVE_PTSNAME@ _GL_FUNCDECL_SYS (ptsname, char *, (int fd)); # endif _GL_CXXALIAS_SYS (ptsname, char *, (int fd)); # endif _GL_CXXALIASWARN (ptsname); #elif defined GNULIB_POSIXCHECK # undef ptsname # if HAVE_RAW_DECL_PTSNAME _GL_WARN_ON_USE (ptsname, "ptsname is not portable - " "use gnulib module ptsname for portability"); # endif #endif #if @GNULIB_PTSNAME_R@ /* Set the pathname of the pseudo-terminal slave associated with the master FD is open on and return 0, or set errno and return non-zero on errors. */ # if @REPLACE_PTSNAME_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ptsname_r # define ptsname_r rpl_ptsname_r # endif _GL_FUNCDECL_RPL (ptsname_r, int, (int fd, char *buf, size_t len)); _GL_CXXALIAS_RPL (ptsname_r, int, (int fd, char *buf, size_t len)); # else # if !@HAVE_PTSNAME_R@ _GL_FUNCDECL_SYS (ptsname_r, int, (int fd, char *buf, size_t len)); # endif _GL_CXXALIAS_SYS (ptsname_r, int, (int fd, char *buf, size_t len)); # endif _GL_CXXALIASWARN (ptsname_r); #elif defined GNULIB_POSIXCHECK # undef ptsname_r # if HAVE_RAW_DECL_PTSNAME_R _GL_WARN_ON_USE (ptsname_r, "ptsname_r is not portable - " "use gnulib module ptsname_r for portability"); # endif #endif #if @GNULIB_PUTENV@ # if @REPLACE_PUTENV@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef putenv # define putenv rpl_putenv # endif _GL_FUNCDECL_RPL (putenv, int, (char *string) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (putenv, int, (char *string)); # else _GL_CXXALIAS_SYS (putenv, int, (char *string)); # endif _GL_CXXALIASWARN (putenv); #endif #if @GNULIB_QSORT_R@ /* Sort an array of NMEMB elements, starting at address BASE, each element occupying SIZE bytes, in ascending order according to the comparison function COMPARE. */ # if @REPLACE_QSORT_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef qsort_r # define qsort_r rpl_qsort_r # endif _GL_FUNCDECL_RPL (qsort_r, void, (void *base, size_t nmemb, size_t size, int (*compare) (void const *, void const *, void *), void *arg) _GL_ARG_NONNULL ((1, 4))); _GL_CXXALIAS_RPL (qsort_r, void, (void *base, size_t nmemb, size_t size, int (*compare) (void const *, void const *, void *), void *arg)); # else # if !@HAVE_QSORT_R@ _GL_FUNCDECL_SYS (qsort_r, void, (void *base, size_t nmemb, size_t size, int (*compare) (void const *, void const *, void *), void *arg) _GL_ARG_NONNULL ((1, 4))); # endif _GL_CXXALIAS_SYS (qsort_r, void, (void *base, size_t nmemb, size_t size, int (*compare) (void const *, void const *, void *), void *arg)); # endif _GL_CXXALIASWARN (qsort_r); #elif defined GNULIB_POSIXCHECK # undef qsort_r # if HAVE_RAW_DECL_QSORT_R _GL_WARN_ON_USE (qsort_r, "qsort_r is not portable - " "use gnulib module qsort_r for portability"); # endif #endif #if @GNULIB_RANDOM_R@ # if !@HAVE_RANDOM_R@ # ifndef RAND_MAX # define RAND_MAX 2147483647 # endif # endif #endif #if @GNULIB_RANDOM@ # if !@HAVE_RANDOM@ _GL_FUNCDECL_SYS (random, long, (void)); # endif _GL_CXXALIAS_SYS (random, long, (void)); _GL_CXXALIASWARN (random); #elif defined GNULIB_POSIXCHECK # undef random # if HAVE_RAW_DECL_RANDOM _GL_WARN_ON_USE (random, "random is unportable - " "use gnulib module random for portability"); # endif #endif #if @GNULIB_RANDOM@ # if !@HAVE_RANDOM@ _GL_FUNCDECL_SYS (srandom, void, (unsigned int seed)); # endif _GL_CXXALIAS_SYS (srandom, void, (unsigned int seed)); _GL_CXXALIASWARN (srandom); #elif defined GNULIB_POSIXCHECK # undef srandom # if HAVE_RAW_DECL_SRANDOM _GL_WARN_ON_USE (srandom, "srandom is unportable - " "use gnulib module random for portability"); # endif #endif #if @GNULIB_RANDOM@ # if !@HAVE_RANDOM@ _GL_FUNCDECL_SYS (initstate, char *, (unsigned int seed, char *buf, size_t buf_size) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (initstate, char *, (unsigned int seed, char *buf, size_t buf_size)); _GL_CXXALIASWARN (initstate); #elif defined GNULIB_POSIXCHECK # undef initstate # if HAVE_RAW_DECL_INITSTATE_R _GL_WARN_ON_USE (initstate, "initstate is unportable - " "use gnulib module random for portability"); # endif #endif #if @GNULIB_RANDOM@ # if !@HAVE_RANDOM@ _GL_FUNCDECL_SYS (setstate, char *, (char *arg_state) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (setstate, char *, (char *arg_state)); _GL_CXXALIASWARN (setstate); #elif defined GNULIB_POSIXCHECK # undef setstate # if HAVE_RAW_DECL_SETSTATE_R _GL_WARN_ON_USE (setstate, "setstate is unportable - " "use gnulib module random for portability"); # endif #endif #if @GNULIB_RANDOM_R@ # if @REPLACE_RANDOM_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef random_r # define random_r rpl_random_r # endif _GL_FUNCDECL_RPL (random_r, int, (struct random_data *buf, int32_t *result) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (random_r, int, (struct random_data *buf, int32_t *result)); # else # if !@HAVE_RANDOM_R@ _GL_FUNCDECL_SYS (random_r, int, (struct random_data *buf, int32_t *result) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (random_r, int, (struct random_data *buf, int32_t *result)); # endif _GL_CXXALIASWARN (random_r); #elif defined GNULIB_POSIXCHECK # undef random_r # if HAVE_RAW_DECL_RANDOM_R _GL_WARN_ON_USE (random_r, "random_r is unportable - " "use gnulib module random_r for portability"); # endif #endif #if @GNULIB_RANDOM_R@ # if @REPLACE_RANDOM_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef srandom_r # define srandom_r rpl_srandom_r # endif _GL_FUNCDECL_RPL (srandom_r, int, (unsigned int seed, struct random_data *rand_state) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (srandom_r, int, (unsigned int seed, struct random_data *rand_state)); # else # if !@HAVE_RANDOM_R@ _GL_FUNCDECL_SYS (srandom_r, int, (unsigned int seed, struct random_data *rand_state) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (srandom_r, int, (unsigned int seed, struct random_data *rand_state)); # endif _GL_CXXALIASWARN (srandom_r); #elif defined GNULIB_POSIXCHECK # undef srandom_r # if HAVE_RAW_DECL_SRANDOM_R _GL_WARN_ON_USE (srandom_r, "srandom_r is unportable - " "use gnulib module random_r for portability"); # endif #endif #if @GNULIB_RANDOM_R@ # if @REPLACE_RANDOM_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef initstate_r # define initstate_r rpl_initstate_r # endif _GL_FUNCDECL_RPL (initstate_r, int, (unsigned int seed, char *buf, size_t buf_size, struct random_data *rand_state) _GL_ARG_NONNULL ((2, 4))); _GL_CXXALIAS_RPL (initstate_r, int, (unsigned int seed, char *buf, size_t buf_size, struct random_data *rand_state)); # else # if !@HAVE_RANDOM_R@ _GL_FUNCDECL_SYS (initstate_r, int, (unsigned int seed, char *buf, size_t buf_size, struct random_data *rand_state) _GL_ARG_NONNULL ((2, 4))); # endif _GL_CXXALIAS_SYS (initstate_r, int, (unsigned int seed, char *buf, size_t buf_size, struct random_data *rand_state)); # endif _GL_CXXALIASWARN (initstate_r); #elif defined GNULIB_POSIXCHECK # undef initstate_r # if HAVE_RAW_DECL_INITSTATE_R _GL_WARN_ON_USE (initstate_r, "initstate_r is unportable - " "use gnulib module random_r for portability"); # endif #endif #if @GNULIB_RANDOM_R@ # if @REPLACE_RANDOM_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef setstate_r # define setstate_r rpl_setstate_r # endif _GL_FUNCDECL_RPL (setstate_r, int, (char *arg_state, struct random_data *rand_state) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (setstate_r, int, (char *arg_state, struct random_data *rand_state)); # else # if !@HAVE_RANDOM_R@ _GL_FUNCDECL_SYS (setstate_r, int, (char *arg_state, struct random_data *rand_state) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (setstate_r, int, (char *arg_state, struct random_data *rand_state)); # endif _GL_CXXALIASWARN (setstate_r); #elif defined GNULIB_POSIXCHECK # undef setstate_r # if HAVE_RAW_DECL_SETSTATE_R _GL_WARN_ON_USE (setstate_r, "setstate_r is unportable - " "use gnulib module random_r for portability"); # endif #endif #if @GNULIB_REALLOC_POSIX@ # if @REPLACE_REALLOC@ # if !((defined __cplusplus && defined GNULIB_NAMESPACE) \ || _GL_USE_STDLIB_ALLOC) # undef realloc # define realloc rpl_realloc # endif _GL_FUNCDECL_RPL (realloc, void *, (void *ptr, size_t size)); _GL_CXXALIAS_RPL (realloc, void *, (void *ptr, size_t size)); # else _GL_CXXALIAS_SYS (realloc, void *, (void *ptr, size_t size)); # endif _GL_CXXALIASWARN (realloc); #elif defined GNULIB_POSIXCHECK && !_GL_USE_STDLIB_ALLOC # undef realloc /* Assume realloc is always declared. */ _GL_WARN_ON_USE (realloc, "realloc is not POSIX compliant everywhere - " "use gnulib module realloc-posix for portability"); #endif #if @GNULIB_REALPATH@ # if @REPLACE_REALPATH@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define realpath rpl_realpath # endif _GL_FUNCDECL_RPL (realpath, char *, (const char *name, char *resolved) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (realpath, char *, (const char *name, char *resolved)); # else # if !@HAVE_REALPATH@ _GL_FUNCDECL_SYS (realpath, char *, (const char *name, char *resolved) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (realpath, char *, (const char *name, char *resolved)); # endif _GL_CXXALIASWARN (realpath); #elif defined GNULIB_POSIXCHECK # undef realpath # if HAVE_RAW_DECL_REALPATH _GL_WARN_ON_USE (realpath, "realpath is unportable - use gnulib module " "canonicalize or canonicalize-lgpl for portability"); # endif #endif #if @GNULIB_RPMATCH@ /* Test a user response to a question. Return 1 if it is affirmative, 0 if it is negative, or -1 if not clear. */ # if !@HAVE_RPMATCH@ _GL_FUNCDECL_SYS (rpmatch, int, (const char *response) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (rpmatch, int, (const char *response)); _GL_CXXALIASWARN (rpmatch); #elif defined GNULIB_POSIXCHECK # undef rpmatch # if HAVE_RAW_DECL_RPMATCH _GL_WARN_ON_USE (rpmatch, "rpmatch is unportable - " "use gnulib module rpmatch for portability"); # endif #endif #if @GNULIB_SECURE_GETENV@ /* Look up NAME in the environment, returning 0 in insecure situations. */ # if !@HAVE_SECURE_GETENV@ _GL_FUNCDECL_SYS (secure_getenv, char *, (char const *name) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (secure_getenv, char *, (char const *name)); _GL_CXXALIASWARN (secure_getenv); #elif defined GNULIB_POSIXCHECK # undef secure_getenv # if HAVE_RAW_DECL_SECURE_GETENV _GL_WARN_ON_USE (secure_getenv, "secure_getenv is unportable - " "use gnulib module secure_getenv for portability"); # endif #endif #if @GNULIB_SETENV@ /* Set NAME to VALUE in the environment. If REPLACE is nonzero, overwrite an existing value. */ # if @REPLACE_SETENV@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef setenv # define setenv rpl_setenv # endif _GL_FUNCDECL_RPL (setenv, int, (const char *name, const char *value, int replace) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (setenv, int, (const char *name, const char *value, int replace)); # else # if !@HAVE_DECL_SETENV@ _GL_FUNCDECL_SYS (setenv, int, (const char *name, const char *value, int replace) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (setenv, int, (const char *name, const char *value, int replace)); # endif # if !(@REPLACE_SETENV@ && !@HAVE_DECL_SETENV@) _GL_CXXALIASWARN (setenv); # endif #elif defined GNULIB_POSIXCHECK # undef setenv # if HAVE_RAW_DECL_SETENV _GL_WARN_ON_USE (setenv, "setenv is unportable - " "use gnulib module setenv for portability"); # endif #endif #if @GNULIB_STRTOD@ /* Parse a double from STRING, updating ENDP if appropriate. */ # if @REPLACE_STRTOD@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define strtod rpl_strtod # endif _GL_FUNCDECL_RPL (strtod, double, (const char *str, char **endp) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (strtod, double, (const char *str, char **endp)); # else # if !@HAVE_STRTOD@ _GL_FUNCDECL_SYS (strtod, double, (const char *str, char **endp) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strtod, double, (const char *str, char **endp)); # endif _GL_CXXALIASWARN (strtod); #elif defined GNULIB_POSIXCHECK # undef strtod # if HAVE_RAW_DECL_STRTOD _GL_WARN_ON_USE (strtod, "strtod is unportable - " "use gnulib module strtod for portability"); # endif #endif #if @GNULIB_STRTOLL@ /* Parse a signed integer whose textual representation starts at STRING. The integer is expected to be in base BASE (2 <= BASE <= 36); if BASE == 0, it may be decimal or octal (with prefix "0") or hexadecimal (with prefix "0x"). If ENDPTR is not NULL, the address of the first byte after the integer is stored in *ENDPTR. Upon overflow, the return value is LLONG_MAX or LLONG_MIN, and errno is set to ERANGE. */ # if !@HAVE_STRTOLL@ _GL_FUNCDECL_SYS (strtoll, long long, (const char *string, char **endptr, int base) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strtoll, long long, (const char *string, char **endptr, int base)); _GL_CXXALIASWARN (strtoll); #elif defined GNULIB_POSIXCHECK # undef strtoll # if HAVE_RAW_DECL_STRTOLL _GL_WARN_ON_USE (strtoll, "strtoll is unportable - " "use gnulib module strtoll for portability"); # endif #endif #if @GNULIB_STRTOULL@ /* Parse an unsigned integer whose textual representation starts at STRING. The integer is expected to be in base BASE (2 <= BASE <= 36); if BASE == 0, it may be decimal or octal (with prefix "0") or hexadecimal (with prefix "0x"). If ENDPTR is not NULL, the address of the first byte after the integer is stored in *ENDPTR. Upon overflow, the return value is ULLONG_MAX, and errno is set to ERANGE. */ # if !@HAVE_STRTOULL@ _GL_FUNCDECL_SYS (strtoull, unsigned long long, (const char *string, char **endptr, int base) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strtoull, unsigned long long, (const char *string, char **endptr, int base)); _GL_CXXALIASWARN (strtoull); #elif defined GNULIB_POSIXCHECK # undef strtoull # if HAVE_RAW_DECL_STRTOULL _GL_WARN_ON_USE (strtoull, "strtoull is unportable - " "use gnulib module strtoull for portability"); # endif #endif #if @GNULIB_UNLOCKPT@ /* Unlock the slave side of the pseudo-terminal whose master side is specified by FD, so that it can be opened. */ # if !@HAVE_UNLOCKPT@ _GL_FUNCDECL_SYS (unlockpt, int, (int fd)); # endif _GL_CXXALIAS_SYS (unlockpt, int, (int fd)); _GL_CXXALIASWARN (unlockpt); #elif defined GNULIB_POSIXCHECK # undef unlockpt # if HAVE_RAW_DECL_UNLOCKPT _GL_WARN_ON_USE (unlockpt, "unlockpt is not portable - " "use gnulib module unlockpt for portability"); # endif #endif #if @GNULIB_UNSETENV@ /* Remove the variable NAME from the environment. */ # if @REPLACE_UNSETENV@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef unsetenv # define unsetenv rpl_unsetenv # endif _GL_FUNCDECL_RPL (unsetenv, int, (const char *name) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (unsetenv, int, (const char *name)); # else # if !@HAVE_DECL_UNSETENV@ _GL_FUNCDECL_SYS (unsetenv, int, (const char *name) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (unsetenv, int, (const char *name)); # endif # if !(@REPLACE_UNSETENV@ && !@HAVE_DECL_UNSETENV@) _GL_CXXALIASWARN (unsetenv); # endif #elif defined GNULIB_POSIXCHECK # undef unsetenv # if HAVE_RAW_DECL_UNSETENV _GL_WARN_ON_USE (unsetenv, "unsetenv is unportable - " "use gnulib module unsetenv for portability"); # endif #endif /* Convert a wide character to a multibyte character. */ #if @GNULIB_WCTOMB@ # if @REPLACE_WCTOMB@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef wctomb # define wctomb rpl_wctomb # endif _GL_FUNCDECL_RPL (wctomb, int, (char *s, wchar_t wc)); _GL_CXXALIAS_RPL (wctomb, int, (char *s, wchar_t wc)); # else _GL_CXXALIAS_SYS (wctomb, int, (char *s, wchar_t wc)); # endif _GL_CXXALIASWARN (wctomb); #endif #endif /* _@GUARD_PREFIX@_STDLIB_H */ #endif /* _@GUARD_PREFIX@_STDLIB_H */ #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/stdio.in.h0000644000175000017500000014256213004436754016311 00000000000000/* A GNU-like . Copyright (C) 2004, 2007-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if defined __need_FILE || defined __need___FILE || defined _GL_ALREADY_INCLUDING_STDIO_H /* Special invocation convention: - Inside glibc header files. - On OSF/1 5.1 we have a sequence of nested includes -> -> -> -> -> -> -> . In this situation, the functions are not yet declared, therefore we cannot provide the C++ aliases. */ #@INCLUDE_NEXT@ @NEXT_STDIO_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_STDIO_H #define _GL_ALREADY_INCLUDING_STDIO_H /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_STDIO_H@ #undef _GL_ALREADY_INCLUDING_STDIO_H #ifndef _@GUARD_PREFIX@_STDIO_H #define _@GUARD_PREFIX@_STDIO_H /* Get va_list. Needed on many systems, including glibc 2.8. */ #include #include /* Get off_t and ssize_t. Needed on many systems, including glibc 2.8 and eglibc 2.11.2. May also define off_t to a 64-bit type on native Windows. */ #include /* The __attribute__ feature is available in gcc versions 2.5 and later. The __-protected variants of the attributes 'format' and 'printf' are accepted by gcc versions 2.6.4 (effectively 2.7) and later. We enable _GL_ATTRIBUTE_FORMAT only if these are supported too, because gnulib and libintl do '#define printf __printf__' when they override the 'printf' function. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 7) # define _GL_ATTRIBUTE_FORMAT(spec) __attribute__ ((__format__ spec)) #else # define _GL_ATTRIBUTE_FORMAT(spec) /* empty */ #endif /* _GL_ATTRIBUTE_FORMAT_PRINTF indicates to GCC that the function takes a format string and arguments, where the format string directives are the ones standardized by ISO C99 and POSIX. */ #if __GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4) # define _GL_ATTRIBUTE_FORMAT_PRINTF(formatstring_parameter, first_argument) \ _GL_ATTRIBUTE_FORMAT ((__gnu_printf__, formatstring_parameter, first_argument)) #else # define _GL_ATTRIBUTE_FORMAT_PRINTF(formatstring_parameter, first_argument) \ _GL_ATTRIBUTE_FORMAT ((__printf__, formatstring_parameter, first_argument)) #endif /* _GL_ATTRIBUTE_FORMAT_PRINTF_SYSTEM is like _GL_ATTRIBUTE_FORMAT_PRINTF, except that it indicates to GCC that the supported format string directives are the ones of the system printf(), rather than the ones standardized by ISO C99 and POSIX. */ #if GNULIB_PRINTF_ATTRIBUTE_FLAVOR_GNU # define _GL_ATTRIBUTE_FORMAT_PRINTF_SYSTEM(formatstring_parameter, first_argument) \ _GL_ATTRIBUTE_FORMAT_PRINTF (formatstring_parameter, first_argument) #else # define _GL_ATTRIBUTE_FORMAT_PRINTF_SYSTEM(formatstring_parameter, first_argument) \ _GL_ATTRIBUTE_FORMAT ((__printf__, formatstring_parameter, first_argument)) #endif /* _GL_ATTRIBUTE_FORMAT_SCANF indicates to GCC that the function takes a format string and arguments, where the format string directives are the ones standardized by ISO C99 and POSIX. */ #if __GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4) # define _GL_ATTRIBUTE_FORMAT_SCANF(formatstring_parameter, first_argument) \ _GL_ATTRIBUTE_FORMAT ((__gnu_scanf__, formatstring_parameter, first_argument)) #else # define _GL_ATTRIBUTE_FORMAT_SCANF(formatstring_parameter, first_argument) \ _GL_ATTRIBUTE_FORMAT ((__scanf__, formatstring_parameter, first_argument)) #endif /* _GL_ATTRIBUTE_FORMAT_SCANF_SYSTEM is like _GL_ATTRIBUTE_FORMAT_SCANF, except that it indicates to GCC that the supported format string directives are the ones of the system scanf(), rather than the ones standardized by ISO C99 and POSIX. */ #define _GL_ATTRIBUTE_FORMAT_SCANF_SYSTEM(formatstring_parameter, first_argument) \ _GL_ATTRIBUTE_FORMAT ((__scanf__, formatstring_parameter, first_argument)) /* Solaris 10 declares renameat in , not in . */ /* But in any case avoid namespace pollution on glibc systems. */ #if (@GNULIB_RENAMEAT@ || defined GNULIB_POSIXCHECK) && defined __sun \ && ! defined __GLIBC__ # include #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Macros for stringification. */ #define _GL_STDIO_STRINGIZE(token) #token #define _GL_STDIO_MACROEXPAND_AND_STRINGIZE(token) _GL_STDIO_STRINGIZE(token) /* When also using extern inline, suppress the use of static inline in standard headers of problematic Apple configurations, as Libc at least through Libc-825.26 (2013-04-09) mishandles it; see, e.g., . Perhaps Apple will fix this some day. */ #if (defined _GL_EXTERN_INLINE_IN_USE && defined __APPLE__ \ && defined __GNUC__ && defined __STDC__) # undef putc_unlocked #endif #if @GNULIB_DPRINTF@ # if @REPLACE_DPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define dprintf rpl_dprintf # endif _GL_FUNCDECL_RPL (dprintf, int, (int fd, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (dprintf, int, (int fd, const char *format, ...)); # else # if !@HAVE_DPRINTF@ _GL_FUNCDECL_SYS (dprintf, int, (int fd, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (dprintf, int, (int fd, const char *format, ...)); # endif _GL_CXXALIASWARN (dprintf); #elif defined GNULIB_POSIXCHECK # undef dprintf # if HAVE_RAW_DECL_DPRINTF _GL_WARN_ON_USE (dprintf, "dprintf is unportable - " "use gnulib module dprintf for portability"); # endif #endif #if @GNULIB_FCLOSE@ /* Close STREAM and its underlying file descriptor. */ # if @REPLACE_FCLOSE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define fclose rpl_fclose # endif _GL_FUNCDECL_RPL (fclose, int, (FILE *stream) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (fclose, int, (FILE *stream)); # else _GL_CXXALIAS_SYS (fclose, int, (FILE *stream)); # endif _GL_CXXALIASWARN (fclose); #elif defined GNULIB_POSIXCHECK # undef fclose /* Assume fclose is always declared. */ _GL_WARN_ON_USE (fclose, "fclose is not always POSIX compliant - " "use gnulib module fclose for portable POSIX compliance"); #endif #if @GNULIB_FDOPEN@ # if @REPLACE_FDOPEN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fdopen # define fdopen rpl_fdopen # endif _GL_FUNCDECL_RPL (fdopen, FILE *, (int fd, const char *mode) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (fdopen, FILE *, (int fd, const char *mode)); # else _GL_CXXALIAS_SYS (fdopen, FILE *, (int fd, const char *mode)); # endif _GL_CXXALIASWARN (fdopen); #elif defined GNULIB_POSIXCHECK # undef fdopen /* Assume fdopen is always declared. */ _GL_WARN_ON_USE (fdopen, "fdopen on native Windows platforms is not POSIX compliant - " "use gnulib module fdopen for portability"); #endif #if @GNULIB_FFLUSH@ /* Flush all pending data on STREAM according to POSIX rules. Both output and seekable input streams are supported. Note! LOSS OF DATA can occur if fflush is applied on an input stream that is _not_seekable_ or on an update stream that is _not_seekable_ and in which the most recent operation was input. Seekability can be tested with lseek(fileno(fp),0,SEEK_CUR). */ # if @REPLACE_FFLUSH@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define fflush rpl_fflush # endif _GL_FUNCDECL_RPL (fflush, int, (FILE *gl_stream)); _GL_CXXALIAS_RPL (fflush, int, (FILE *gl_stream)); # else _GL_CXXALIAS_SYS (fflush, int, (FILE *gl_stream)); # endif _GL_CXXALIASWARN (fflush); #elif defined GNULIB_POSIXCHECK # undef fflush /* Assume fflush is always declared. */ _GL_WARN_ON_USE (fflush, "fflush is not always POSIX compliant - " "use gnulib module fflush for portable POSIX compliance"); #endif #if @GNULIB_FGETC@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fgetc # define fgetc rpl_fgetc # endif _GL_FUNCDECL_RPL (fgetc, int, (FILE *stream) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (fgetc, int, (FILE *stream)); # else _GL_CXXALIAS_SYS (fgetc, int, (FILE *stream)); # endif _GL_CXXALIASWARN (fgetc); #endif #if @GNULIB_FGETS@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fgets # define fgets rpl_fgets # endif _GL_FUNCDECL_RPL (fgets, char *, (char *s, int n, FILE *stream) _GL_ARG_NONNULL ((1, 3))); _GL_CXXALIAS_RPL (fgets, char *, (char *s, int n, FILE *stream)); # else _GL_CXXALIAS_SYS (fgets, char *, (char *s, int n, FILE *stream)); # endif _GL_CXXALIASWARN (fgets); #endif #if @GNULIB_FOPEN@ # if @REPLACE_FOPEN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fopen # define fopen rpl_fopen # endif _GL_FUNCDECL_RPL (fopen, FILE *, (const char *filename, const char *mode) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (fopen, FILE *, (const char *filename, const char *mode)); # else _GL_CXXALIAS_SYS (fopen, FILE *, (const char *filename, const char *mode)); # endif _GL_CXXALIASWARN (fopen); #elif defined GNULIB_POSIXCHECK # undef fopen /* Assume fopen is always declared. */ _GL_WARN_ON_USE (fopen, "fopen on native Windows platforms is not POSIX compliant - " "use gnulib module fopen for portability"); #endif #if @GNULIB_FPRINTF_POSIX@ || @GNULIB_FPRINTF@ # if (@GNULIB_FPRINTF_POSIX@ && @REPLACE_FPRINTF@) \ || (@GNULIB_FPRINTF@ && @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@)) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define fprintf rpl_fprintf # endif # define GNULIB_overrides_fprintf 1 # if @GNULIB_FPRINTF_POSIX@ || @GNULIB_VFPRINTF_POSIX@ _GL_FUNCDECL_RPL (fprintf, int, (FILE *fp, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((1, 2))); # else _GL_FUNCDECL_RPL (fprintf, int, (FILE *fp, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF_SYSTEM (2, 3) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_RPL (fprintf, int, (FILE *fp, const char *format, ...)); # else _GL_CXXALIAS_SYS (fprintf, int, (FILE *fp, const char *format, ...)); # endif _GL_CXXALIASWARN (fprintf); #endif #if !@GNULIB_FPRINTF_POSIX@ && defined GNULIB_POSIXCHECK # if !GNULIB_overrides_fprintf # undef fprintf # endif /* Assume fprintf is always declared. */ _GL_WARN_ON_USE (fprintf, "fprintf is not always POSIX compliant - " "use gnulib module fprintf-posix for portable " "POSIX compliance"); #endif #if @GNULIB_FPURGE@ /* Discard all pending buffered I/O data on STREAM. STREAM must not be wide-character oriented. When discarding pending output, the file position is set back to where it was before the write calls. When discarding pending input, the file position is advanced to match the end of the previously read input. Return 0 if successful. Upon error, return -1 and set errno. */ # if @REPLACE_FPURGE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define fpurge rpl_fpurge # endif _GL_FUNCDECL_RPL (fpurge, int, (FILE *gl_stream) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (fpurge, int, (FILE *gl_stream)); # else # if !@HAVE_DECL_FPURGE@ _GL_FUNCDECL_SYS (fpurge, int, (FILE *gl_stream) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (fpurge, int, (FILE *gl_stream)); # endif _GL_CXXALIASWARN (fpurge); #elif defined GNULIB_POSIXCHECK # undef fpurge # if HAVE_RAW_DECL_FPURGE _GL_WARN_ON_USE (fpurge, "fpurge is not always present - " "use gnulib module fpurge for portability"); # endif #endif #if @GNULIB_FPUTC@ # if @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fputc # define fputc rpl_fputc # endif _GL_FUNCDECL_RPL (fputc, int, (int c, FILE *stream) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (fputc, int, (int c, FILE *stream)); # else _GL_CXXALIAS_SYS (fputc, int, (int c, FILE *stream)); # endif _GL_CXXALIASWARN (fputc); #endif #if @GNULIB_FPUTS@ # if @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fputs # define fputs rpl_fputs # endif _GL_FUNCDECL_RPL (fputs, int, (const char *string, FILE *stream) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (fputs, int, (const char *string, FILE *stream)); # else _GL_CXXALIAS_SYS (fputs, int, (const char *string, FILE *stream)); # endif _GL_CXXALIASWARN (fputs); #endif #if @GNULIB_FREAD@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fread # define fread rpl_fread # endif _GL_FUNCDECL_RPL (fread, size_t, (void *ptr, size_t s, size_t n, FILE *stream) _GL_ARG_NONNULL ((4))); _GL_CXXALIAS_RPL (fread, size_t, (void *ptr, size_t s, size_t n, FILE *stream)); # else _GL_CXXALIAS_SYS (fread, size_t, (void *ptr, size_t s, size_t n, FILE *stream)); # endif _GL_CXXALIASWARN (fread); #endif #if @GNULIB_FREOPEN@ # if @REPLACE_FREOPEN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef freopen # define freopen rpl_freopen # endif _GL_FUNCDECL_RPL (freopen, FILE *, (const char *filename, const char *mode, FILE *stream) _GL_ARG_NONNULL ((2, 3))); _GL_CXXALIAS_RPL (freopen, FILE *, (const char *filename, const char *mode, FILE *stream)); # else _GL_CXXALIAS_SYS (freopen, FILE *, (const char *filename, const char *mode, FILE *stream)); # endif _GL_CXXALIASWARN (freopen); #elif defined GNULIB_POSIXCHECK # undef freopen /* Assume freopen is always declared. */ _GL_WARN_ON_USE (freopen, "freopen on native Windows platforms is not POSIX compliant - " "use gnulib module freopen for portability"); #endif #if @GNULIB_FSCANF@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fscanf # define fscanf rpl_fscanf # endif _GL_FUNCDECL_RPL (fscanf, int, (FILE *stream, const char *format, ...) _GL_ATTRIBUTE_FORMAT_SCANF_SYSTEM (2, 3) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (fscanf, int, (FILE *stream, const char *format, ...)); # else _GL_CXXALIAS_SYS (fscanf, int, (FILE *stream, const char *format, ...)); # endif _GL_CXXALIASWARN (fscanf); #endif /* Set up the following warnings, based on which modules are in use. GNU Coding Standards discourage the use of fseek, since it imposes an arbitrary limitation on some 32-bit hosts. Remember that the fseek module depends on the fseeko module, so we only have three cases to consider: 1. The developer is not using either module. Issue a warning under GNULIB_POSIXCHECK for both functions, to remind them that both functions have bugs on some systems. _GL_NO_LARGE_FILES has no impact on this warning. 2. The developer is using both modules. They may be unaware of the arbitrary limitations of fseek, so issue a warning under GNULIB_POSIXCHECK. On the other hand, they may be using both modules intentionally, so the developer can define _GL_NO_LARGE_FILES in the compilation units where the use of fseek is safe, to silence the warning. 3. The developer is using the fseeko module, but not fseek. Gnulib guarantees that fseek will still work around platform bugs in that case, but we presume that the developer is aware of the pitfalls of fseek and was trying to avoid it, so issue a warning even when GNULIB_POSIXCHECK is undefined. Again, _GL_NO_LARGE_FILES can be defined to silence the warning in particular compilation units. In C++ compilations with GNULIB_NAMESPACE, in order to avoid that fseek gets defined as a macro, it is recommended that the developer uses the fseek module, even if he is not calling the fseek function. Most gnulib clients that perform stream operations should fall into category 3. */ #if @GNULIB_FSEEK@ # if defined GNULIB_POSIXCHECK && !defined _GL_NO_LARGE_FILES # define _GL_FSEEK_WARN /* Category 2, above. */ # undef fseek # endif # if @REPLACE_FSEEK@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fseek # define fseek rpl_fseek # endif _GL_FUNCDECL_RPL (fseek, int, (FILE *fp, long offset, int whence) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (fseek, int, (FILE *fp, long offset, int whence)); # else _GL_CXXALIAS_SYS (fseek, int, (FILE *fp, long offset, int whence)); # endif _GL_CXXALIASWARN (fseek); #endif #if @GNULIB_FSEEKO@ # if !@GNULIB_FSEEK@ && !defined _GL_NO_LARGE_FILES # define _GL_FSEEK_WARN /* Category 3, above. */ # undef fseek # endif # if @REPLACE_FSEEKO@ /* Provide an fseeko function that is aware of a preceding fflush(), and which detects pipes. */ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fseeko # define fseeko rpl_fseeko # endif _GL_FUNCDECL_RPL (fseeko, int, (FILE *fp, off_t offset, int whence) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (fseeko, int, (FILE *fp, off_t offset, int whence)); # else # if ! @HAVE_DECL_FSEEKO@ _GL_FUNCDECL_SYS (fseeko, int, (FILE *fp, off_t offset, int whence) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (fseeko, int, (FILE *fp, off_t offset, int whence)); # endif _GL_CXXALIASWARN (fseeko); #elif defined GNULIB_POSIXCHECK # define _GL_FSEEK_WARN /* Category 1, above. */ # undef fseek # undef fseeko # if HAVE_RAW_DECL_FSEEKO _GL_WARN_ON_USE (fseeko, "fseeko is unportable - " "use gnulib module fseeko for portability"); # endif #endif #ifdef _GL_FSEEK_WARN # undef _GL_FSEEK_WARN /* Here, either fseek is undefined (but C89 guarantees that it is declared), or it is defined as rpl_fseek (declared above). */ _GL_WARN_ON_USE (fseek, "fseek cannot handle files larger than 4 GB " "on 32-bit platforms - " "use fseeko function for handling of large files"); #endif /* ftell, ftello. See the comments on fseek/fseeko. */ #if @GNULIB_FTELL@ # if defined GNULIB_POSIXCHECK && !defined _GL_NO_LARGE_FILES # define _GL_FTELL_WARN /* Category 2, above. */ # undef ftell # endif # if @REPLACE_FTELL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ftell # define ftell rpl_ftell # endif _GL_FUNCDECL_RPL (ftell, long, (FILE *fp) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (ftell, long, (FILE *fp)); # else _GL_CXXALIAS_SYS (ftell, long, (FILE *fp)); # endif _GL_CXXALIASWARN (ftell); #endif #if @GNULIB_FTELLO@ # if !@GNULIB_FTELL@ && !defined _GL_NO_LARGE_FILES # define _GL_FTELL_WARN /* Category 3, above. */ # undef ftell # endif # if @REPLACE_FTELLO@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ftello # define ftello rpl_ftello # endif _GL_FUNCDECL_RPL (ftello, off_t, (FILE *fp) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (ftello, off_t, (FILE *fp)); # else # if ! @HAVE_DECL_FTELLO@ _GL_FUNCDECL_SYS (ftello, off_t, (FILE *fp) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (ftello, off_t, (FILE *fp)); # endif _GL_CXXALIASWARN (ftello); #elif defined GNULIB_POSIXCHECK # define _GL_FTELL_WARN /* Category 1, above. */ # undef ftell # undef ftello # if HAVE_RAW_DECL_FTELLO _GL_WARN_ON_USE (ftello, "ftello is unportable - " "use gnulib module ftello for portability"); # endif #endif #ifdef _GL_FTELL_WARN # undef _GL_FTELL_WARN /* Here, either ftell is undefined (but C89 guarantees that it is declared), or it is defined as rpl_ftell (declared above). */ _GL_WARN_ON_USE (ftell, "ftell cannot handle files larger than 4 GB " "on 32-bit platforms - " "use ftello function for handling of large files"); #endif #if @GNULIB_FWRITE@ # if @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fwrite # define fwrite rpl_fwrite # endif _GL_FUNCDECL_RPL (fwrite, size_t, (const void *ptr, size_t s, size_t n, FILE *stream) _GL_ARG_NONNULL ((1, 4))); _GL_CXXALIAS_RPL (fwrite, size_t, (const void *ptr, size_t s, size_t n, FILE *stream)); # else _GL_CXXALIAS_SYS (fwrite, size_t, (const void *ptr, size_t s, size_t n, FILE *stream)); /* Work around bug 11959 when fortifying glibc 2.4 through 2.15 , which sometimes causes an unwanted diagnostic for fwrite calls. This affects only function declaration attributes under certain versions of gcc and clang, and is not needed for C++. */ # if (0 < __USE_FORTIFY_LEVEL \ && __GLIBC__ == 2 && 4 <= __GLIBC_MINOR__ && __GLIBC_MINOR__ <= 15 \ && 3 < __GNUC__ + (4 <= __GNUC_MINOR__) \ && !defined __cplusplus) # undef fwrite # undef fwrite_unlocked extern size_t __REDIRECT (rpl_fwrite, (const void *__restrict, size_t, size_t, FILE *__restrict), fwrite); extern size_t __REDIRECT (rpl_fwrite_unlocked, (const void *__restrict, size_t, size_t, FILE *__restrict), fwrite_unlocked); # define fwrite rpl_fwrite # define fwrite_unlocked rpl_fwrite_unlocked # endif # endif _GL_CXXALIASWARN (fwrite); #endif #if @GNULIB_GETC@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getc # define getc rpl_fgetc # endif _GL_FUNCDECL_RPL (fgetc, int, (FILE *stream) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL_1 (getc, rpl_fgetc, int, (FILE *stream)); # else _GL_CXXALIAS_SYS (getc, int, (FILE *stream)); # endif _GL_CXXALIASWARN (getc); #endif #if @GNULIB_GETCHAR@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getchar # define getchar rpl_getchar # endif _GL_FUNCDECL_RPL (getchar, int, (void)); _GL_CXXALIAS_RPL (getchar, int, (void)); # else _GL_CXXALIAS_SYS (getchar, int, (void)); # endif _GL_CXXALIASWARN (getchar); #endif #if @GNULIB_GETDELIM@ /* Read input, up to (and including) the next occurrence of DELIMITER, from STREAM, store it in *LINEPTR (and NUL-terminate it). *LINEPTR is a pointer returned from malloc (or NULL), pointing to *LINESIZE bytes of space. It is realloc'd as necessary. Return the number of bytes read and stored at *LINEPTR (not including the NUL terminator), or -1 on error or EOF. */ # if @REPLACE_GETDELIM@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getdelim # define getdelim rpl_getdelim # endif _GL_FUNCDECL_RPL (getdelim, ssize_t, (char **lineptr, size_t *linesize, int delimiter, FILE *stream) _GL_ARG_NONNULL ((1, 2, 4))); _GL_CXXALIAS_RPL (getdelim, ssize_t, (char **lineptr, size_t *linesize, int delimiter, FILE *stream)); # else # if !@HAVE_DECL_GETDELIM@ _GL_FUNCDECL_SYS (getdelim, ssize_t, (char **lineptr, size_t *linesize, int delimiter, FILE *stream) _GL_ARG_NONNULL ((1, 2, 4))); # endif _GL_CXXALIAS_SYS (getdelim, ssize_t, (char **lineptr, size_t *linesize, int delimiter, FILE *stream)); # endif _GL_CXXALIASWARN (getdelim); #elif defined GNULIB_POSIXCHECK # undef getdelim # if HAVE_RAW_DECL_GETDELIM _GL_WARN_ON_USE (getdelim, "getdelim is unportable - " "use gnulib module getdelim for portability"); # endif #endif #if @GNULIB_GETLINE@ /* Read a line, up to (and including) the next newline, from STREAM, store it in *LINEPTR (and NUL-terminate it). *LINEPTR is a pointer returned from malloc (or NULL), pointing to *LINESIZE bytes of space. It is realloc'd as necessary. Return the number of bytes read and stored at *LINEPTR (not including the NUL terminator), or -1 on error or EOF. */ # if @REPLACE_GETLINE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getline # define getline rpl_getline # endif _GL_FUNCDECL_RPL (getline, ssize_t, (char **lineptr, size_t *linesize, FILE *stream) _GL_ARG_NONNULL ((1, 2, 3))); _GL_CXXALIAS_RPL (getline, ssize_t, (char **lineptr, size_t *linesize, FILE *stream)); # else # if !@HAVE_DECL_GETLINE@ _GL_FUNCDECL_SYS (getline, ssize_t, (char **lineptr, size_t *linesize, FILE *stream) _GL_ARG_NONNULL ((1, 2, 3))); # endif _GL_CXXALIAS_SYS (getline, ssize_t, (char **lineptr, size_t *linesize, FILE *stream)); # endif # if @HAVE_DECL_GETLINE@ _GL_CXXALIASWARN (getline); # endif #elif defined GNULIB_POSIXCHECK # undef getline # if HAVE_RAW_DECL_GETLINE _GL_WARN_ON_USE (getline, "getline is unportable - " "use gnulib module getline for portability"); # endif #endif /* It is very rare that the developer ever has full control of stdin, so any use of gets warrants an unconditional warning; besides, C11 removed it. */ #undef gets #if HAVE_RAW_DECL_GETS && !defined __cplusplus _GL_WARN_ON_USE (gets, "gets is a security hole - use fgets instead"); #endif #if @GNULIB_OBSTACK_PRINTF@ || @GNULIB_OBSTACK_PRINTF_POSIX@ struct obstack; /* Grow an obstack with formatted output. Return the number of bytes added to OBS. No trailing nul byte is added, and the object should be closed with obstack_finish before use. Upon memory allocation error, call obstack_alloc_failed_handler. Upon other error, return -1. */ # if @REPLACE_OBSTACK_PRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define obstack_printf rpl_obstack_printf # endif _GL_FUNCDECL_RPL (obstack_printf, int, (struct obstack *obs, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (obstack_printf, int, (struct obstack *obs, const char *format, ...)); # else # if !@HAVE_DECL_OBSTACK_PRINTF@ _GL_FUNCDECL_SYS (obstack_printf, int, (struct obstack *obs, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (obstack_printf, int, (struct obstack *obs, const char *format, ...)); # endif _GL_CXXALIASWARN (obstack_printf); # if @REPLACE_OBSTACK_PRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define obstack_vprintf rpl_obstack_vprintf # endif _GL_FUNCDECL_RPL (obstack_vprintf, int, (struct obstack *obs, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (obstack_vprintf, int, (struct obstack *obs, const char *format, va_list args)); # else # if !@HAVE_DECL_OBSTACK_PRINTF@ _GL_FUNCDECL_SYS (obstack_vprintf, int, (struct obstack *obs, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (obstack_vprintf, int, (struct obstack *obs, const char *format, va_list args)); # endif _GL_CXXALIASWARN (obstack_vprintf); #endif #if @GNULIB_PCLOSE@ # if !@HAVE_PCLOSE@ _GL_FUNCDECL_SYS (pclose, int, (FILE *stream) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (pclose, int, (FILE *stream)); _GL_CXXALIASWARN (pclose); #elif defined GNULIB_POSIXCHECK # undef pclose # if HAVE_RAW_DECL_PCLOSE _GL_WARN_ON_USE (pclose, "pclose is unportable - " "use gnulib module pclose for more portability"); # endif #endif #if @GNULIB_PERROR@ /* Print a message to standard error, describing the value of ERRNO, (if STRING is not NULL and not empty) prefixed with STRING and ": ", and terminated with a newline. */ # if @REPLACE_PERROR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define perror rpl_perror # endif _GL_FUNCDECL_RPL (perror, void, (const char *string)); _GL_CXXALIAS_RPL (perror, void, (const char *string)); # else _GL_CXXALIAS_SYS (perror, void, (const char *string)); # endif _GL_CXXALIASWARN (perror); #elif defined GNULIB_POSIXCHECK # undef perror /* Assume perror is always declared. */ _GL_WARN_ON_USE (perror, "perror is not always POSIX compliant - " "use gnulib module perror for portability"); #endif #if @GNULIB_POPEN@ # if @REPLACE_POPEN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef popen # define popen rpl_popen # endif _GL_FUNCDECL_RPL (popen, FILE *, (const char *cmd, const char *mode) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (popen, FILE *, (const char *cmd, const char *mode)); # else # if !@HAVE_POPEN@ _GL_FUNCDECL_SYS (popen, FILE *, (const char *cmd, const char *mode) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (popen, FILE *, (const char *cmd, const char *mode)); # endif _GL_CXXALIASWARN (popen); #elif defined GNULIB_POSIXCHECK # undef popen # if HAVE_RAW_DECL_POPEN _GL_WARN_ON_USE (popen, "popen is buggy on some platforms - " "use gnulib module popen or pipe for more portability"); # endif #endif #if @GNULIB_PRINTF_POSIX@ || @GNULIB_PRINTF@ # if (@GNULIB_PRINTF_POSIX@ && @REPLACE_PRINTF@) \ || (@GNULIB_PRINTF@ && @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@)) # if defined __GNUC__ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) /* Don't break __attribute__((format(printf,M,N))). */ # define printf __printf__ # endif # if @GNULIB_PRINTF_POSIX@ || @GNULIB_VFPRINTF_POSIX@ _GL_FUNCDECL_RPL_1 (__printf__, int, (const char *format, ...) __asm__ (@ASM_SYMBOL_PREFIX@ _GL_STDIO_MACROEXPAND_AND_STRINGIZE(rpl_printf)) _GL_ATTRIBUTE_FORMAT_PRINTF (1, 2) _GL_ARG_NONNULL ((1))); # else _GL_FUNCDECL_RPL_1 (__printf__, int, (const char *format, ...) __asm__ (@ASM_SYMBOL_PREFIX@ _GL_STDIO_MACROEXPAND_AND_STRINGIZE(rpl_printf)) _GL_ATTRIBUTE_FORMAT_PRINTF_SYSTEM (1, 2) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_RPL_1 (printf, __printf__, int, (const char *format, ...)); # else # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define printf rpl_printf # endif _GL_FUNCDECL_RPL (printf, int, (const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (1, 2) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (printf, int, (const char *format, ...)); # endif # define GNULIB_overrides_printf 1 # else _GL_CXXALIAS_SYS (printf, int, (const char *format, ...)); # endif _GL_CXXALIASWARN (printf); #endif #if !@GNULIB_PRINTF_POSIX@ && defined GNULIB_POSIXCHECK # if !GNULIB_overrides_printf # undef printf # endif /* Assume printf is always declared. */ _GL_WARN_ON_USE (printf, "printf is not always POSIX compliant - " "use gnulib module printf-posix for portable " "POSIX compliance"); #endif #if @GNULIB_PUTC@ # if @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef putc # define putc rpl_fputc # endif _GL_FUNCDECL_RPL (fputc, int, (int c, FILE *stream) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL_1 (putc, rpl_fputc, int, (int c, FILE *stream)); # else _GL_CXXALIAS_SYS (putc, int, (int c, FILE *stream)); # endif _GL_CXXALIASWARN (putc); #endif #if @GNULIB_PUTCHAR@ # if @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef putchar # define putchar rpl_putchar # endif _GL_FUNCDECL_RPL (putchar, int, (int c)); _GL_CXXALIAS_RPL (putchar, int, (int c)); # else _GL_CXXALIAS_SYS (putchar, int, (int c)); # endif _GL_CXXALIASWARN (putchar); #endif #if @GNULIB_PUTS@ # if @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef puts # define puts rpl_puts # endif _GL_FUNCDECL_RPL (puts, int, (const char *string) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (puts, int, (const char *string)); # else _GL_CXXALIAS_SYS (puts, int, (const char *string)); # endif _GL_CXXALIASWARN (puts); #endif #if @GNULIB_REMOVE@ # if @REPLACE_REMOVE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef remove # define remove rpl_remove # endif _GL_FUNCDECL_RPL (remove, int, (const char *name) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (remove, int, (const char *name)); # else _GL_CXXALIAS_SYS (remove, int, (const char *name)); # endif _GL_CXXALIASWARN (remove); #elif defined GNULIB_POSIXCHECK # undef remove /* Assume remove is always declared. */ _GL_WARN_ON_USE (remove, "remove cannot handle directories on some platforms - " "use gnulib module remove for more portability"); #endif #if @GNULIB_RENAME@ # if @REPLACE_RENAME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef rename # define rename rpl_rename # endif _GL_FUNCDECL_RPL (rename, int, (const char *old_filename, const char *new_filename) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (rename, int, (const char *old_filename, const char *new_filename)); # else _GL_CXXALIAS_SYS (rename, int, (const char *old_filename, const char *new_filename)); # endif _GL_CXXALIASWARN (rename); #elif defined GNULIB_POSIXCHECK # undef rename /* Assume rename is always declared. */ _GL_WARN_ON_USE (rename, "rename is buggy on some platforms - " "use gnulib module rename for more portability"); #endif #if @GNULIB_RENAMEAT@ # if @REPLACE_RENAMEAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef renameat # define renameat rpl_renameat # endif _GL_FUNCDECL_RPL (renameat, int, (int fd1, char const *file1, int fd2, char const *file2) _GL_ARG_NONNULL ((2, 4))); _GL_CXXALIAS_RPL (renameat, int, (int fd1, char const *file1, int fd2, char const *file2)); # else # if !@HAVE_RENAMEAT@ _GL_FUNCDECL_SYS (renameat, int, (int fd1, char const *file1, int fd2, char const *file2) _GL_ARG_NONNULL ((2, 4))); # endif _GL_CXXALIAS_SYS (renameat, int, (int fd1, char const *file1, int fd2, char const *file2)); # endif _GL_CXXALIASWARN (renameat); #elif defined GNULIB_POSIXCHECK # undef renameat # if HAVE_RAW_DECL_RENAMEAT _GL_WARN_ON_USE (renameat, "renameat is not portable - " "use gnulib module renameat for portability"); # endif #endif #if @GNULIB_SCANF@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if defined __GNUC__ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef scanf /* Don't break __attribute__((format(scanf,M,N))). */ # define scanf __scanf__ # endif _GL_FUNCDECL_RPL_1 (__scanf__, int, (const char *format, ...) __asm__ (@ASM_SYMBOL_PREFIX@ _GL_STDIO_MACROEXPAND_AND_STRINGIZE(rpl_scanf)) _GL_ATTRIBUTE_FORMAT_SCANF_SYSTEM (1, 2) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL_1 (scanf, __scanf__, int, (const char *format, ...)); # else # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef scanf # define scanf rpl_scanf # endif _GL_FUNCDECL_RPL (scanf, int, (const char *format, ...) _GL_ATTRIBUTE_FORMAT_SCANF_SYSTEM (1, 2) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (scanf, int, (const char *format, ...)); # endif # else _GL_CXXALIAS_SYS (scanf, int, (const char *format, ...)); # endif _GL_CXXALIASWARN (scanf); #endif #if @GNULIB_SNPRINTF@ # if @REPLACE_SNPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define snprintf rpl_snprintf # endif _GL_FUNCDECL_RPL (snprintf, int, (char *str, size_t size, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (3, 4) _GL_ARG_NONNULL ((3))); _GL_CXXALIAS_RPL (snprintf, int, (char *str, size_t size, const char *format, ...)); # else # if !@HAVE_DECL_SNPRINTF@ _GL_FUNCDECL_SYS (snprintf, int, (char *str, size_t size, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (3, 4) _GL_ARG_NONNULL ((3))); # endif _GL_CXXALIAS_SYS (snprintf, int, (char *str, size_t size, const char *format, ...)); # endif _GL_CXXALIASWARN (snprintf); #elif defined GNULIB_POSIXCHECK # undef snprintf # if HAVE_RAW_DECL_SNPRINTF _GL_WARN_ON_USE (snprintf, "snprintf is unportable - " "use gnulib module snprintf for portability"); # endif #endif /* Some people would argue that all sprintf uses should be warned about (for example, OpenBSD issues a link warning for it), since it can cause security holes due to buffer overruns. However, we believe that sprintf can be used safely, and is more efficient than snprintf in those safe cases; and as proof of our belief, we use sprintf in several gnulib modules. So this header intentionally avoids adding a warning to sprintf except when GNULIB_POSIXCHECK is defined. */ #if @GNULIB_SPRINTF_POSIX@ # if @REPLACE_SPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define sprintf rpl_sprintf # endif _GL_FUNCDECL_RPL (sprintf, int, (char *str, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (sprintf, int, (char *str, const char *format, ...)); # else _GL_CXXALIAS_SYS (sprintf, int, (char *str, const char *format, ...)); # endif _GL_CXXALIASWARN (sprintf); #elif defined GNULIB_POSIXCHECK # undef sprintf /* Assume sprintf is always declared. */ _GL_WARN_ON_USE (sprintf, "sprintf is not always POSIX compliant - " "use gnulib module sprintf-posix for portable " "POSIX compliance"); #endif #if @GNULIB_TMPFILE@ # if @REPLACE_TMPFILE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define tmpfile rpl_tmpfile # endif _GL_FUNCDECL_RPL (tmpfile, FILE *, (void)); _GL_CXXALIAS_RPL (tmpfile, FILE *, (void)); # else _GL_CXXALIAS_SYS (tmpfile, FILE *, (void)); # endif _GL_CXXALIASWARN (tmpfile); #elif defined GNULIB_POSIXCHECK # undef tmpfile # if HAVE_RAW_DECL_TMPFILE _GL_WARN_ON_USE (tmpfile, "tmpfile is not usable on mingw - " "use gnulib module tmpfile for portability"); # endif #endif #if @GNULIB_VASPRINTF@ /* Write formatted output to a string dynamically allocated with malloc(). If the memory allocation succeeds, store the address of the string in *RESULT and return the number of resulting bytes, excluding the trailing NUL. Upon memory allocation error, or some other error, return -1. */ # if @REPLACE_VASPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define asprintf rpl_asprintf # endif _GL_FUNCDECL_RPL (asprintf, int, (char **result, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (asprintf, int, (char **result, const char *format, ...)); # else # if !@HAVE_VASPRINTF@ _GL_FUNCDECL_SYS (asprintf, int, (char **result, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (asprintf, int, (char **result, const char *format, ...)); # endif _GL_CXXALIASWARN (asprintf); # if @REPLACE_VASPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define vasprintf rpl_vasprintf # endif _GL_FUNCDECL_RPL (vasprintf, int, (char **result, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (vasprintf, int, (char **result, const char *format, va_list args)); # else # if !@HAVE_VASPRINTF@ _GL_FUNCDECL_SYS (vasprintf, int, (char **result, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (vasprintf, int, (char **result, const char *format, va_list args)); # endif _GL_CXXALIASWARN (vasprintf); #endif #if @GNULIB_VDPRINTF@ # if @REPLACE_VDPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define vdprintf rpl_vdprintf # endif _GL_FUNCDECL_RPL (vdprintf, int, (int fd, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (vdprintf, int, (int fd, const char *format, va_list args)); # else # if !@HAVE_VDPRINTF@ _GL_FUNCDECL_SYS (vdprintf, int, (int fd, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((2))); # endif /* Need to cast, because on Solaris, the third parameter will likely be __va_list args. */ _GL_CXXALIAS_SYS_CAST (vdprintf, int, (int fd, const char *format, va_list args)); # endif _GL_CXXALIASWARN (vdprintf); #elif defined GNULIB_POSIXCHECK # undef vdprintf # if HAVE_RAW_DECL_VDPRINTF _GL_WARN_ON_USE (vdprintf, "vdprintf is unportable - " "use gnulib module vdprintf for portability"); # endif #endif #if @GNULIB_VFPRINTF_POSIX@ || @GNULIB_VFPRINTF@ # if (@GNULIB_VFPRINTF_POSIX@ && @REPLACE_VFPRINTF@) \ || (@GNULIB_VFPRINTF@ && @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@)) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define vfprintf rpl_vfprintf # endif # define GNULIB_overrides_vfprintf 1 # if @GNULIB_VFPRINTF_POSIX@ _GL_FUNCDECL_RPL (vfprintf, int, (FILE *fp, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((1, 2))); # else _GL_FUNCDECL_RPL (vfprintf, int, (FILE *fp, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF_SYSTEM (2, 0) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_RPL (vfprintf, int, (FILE *fp, const char *format, va_list args)); # else /* Need to cast, because on Solaris, the third parameter is __va_list args and GCC's fixincludes did not change this to __gnuc_va_list. */ _GL_CXXALIAS_SYS_CAST (vfprintf, int, (FILE *fp, const char *format, va_list args)); # endif _GL_CXXALIASWARN (vfprintf); #endif #if !@GNULIB_VFPRINTF_POSIX@ && defined GNULIB_POSIXCHECK # if !GNULIB_overrides_vfprintf # undef vfprintf # endif /* Assume vfprintf is always declared. */ _GL_WARN_ON_USE (vfprintf, "vfprintf is not always POSIX compliant - " "use gnulib module vfprintf-posix for portable " "POSIX compliance"); #endif #if @GNULIB_VFSCANF@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef vfscanf # define vfscanf rpl_vfscanf # endif _GL_FUNCDECL_RPL (vfscanf, int, (FILE *stream, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_SCANF_SYSTEM (2, 0) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (vfscanf, int, (FILE *stream, const char *format, va_list args)); # else _GL_CXXALIAS_SYS (vfscanf, int, (FILE *stream, const char *format, va_list args)); # endif _GL_CXXALIASWARN (vfscanf); #endif #if @GNULIB_VPRINTF_POSIX@ || @GNULIB_VPRINTF@ # if (@GNULIB_VPRINTF_POSIX@ && @REPLACE_VPRINTF@) \ || (@GNULIB_VPRINTF@ && @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@)) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define vprintf rpl_vprintf # endif # define GNULIB_overrides_vprintf 1 # if @GNULIB_VPRINTF_POSIX@ || @GNULIB_VFPRINTF_POSIX@ _GL_FUNCDECL_RPL (vprintf, int, (const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (1, 0) _GL_ARG_NONNULL ((1))); # else _GL_FUNCDECL_RPL (vprintf, int, (const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF_SYSTEM (1, 0) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_RPL (vprintf, int, (const char *format, va_list args)); # else /* Need to cast, because on Solaris, the second parameter is __va_list args and GCC's fixincludes did not change this to __gnuc_va_list. */ _GL_CXXALIAS_SYS_CAST (vprintf, int, (const char *format, va_list args)); # endif _GL_CXXALIASWARN (vprintf); #endif #if !@GNULIB_VPRINTF_POSIX@ && defined GNULIB_POSIXCHECK # if !GNULIB_overrides_vprintf # undef vprintf # endif /* Assume vprintf is always declared. */ _GL_WARN_ON_USE (vprintf, "vprintf is not always POSIX compliant - " "use gnulib module vprintf-posix for portable " "POSIX compliance"); #endif #if @GNULIB_VSCANF@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef vscanf # define vscanf rpl_vscanf # endif _GL_FUNCDECL_RPL (vscanf, int, (const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_SCANF_SYSTEM (1, 0) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (vscanf, int, (const char *format, va_list args)); # else _GL_CXXALIAS_SYS (vscanf, int, (const char *format, va_list args)); # endif _GL_CXXALIASWARN (vscanf); #endif #if @GNULIB_VSNPRINTF@ # if @REPLACE_VSNPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define vsnprintf rpl_vsnprintf # endif _GL_FUNCDECL_RPL (vsnprintf, int, (char *str, size_t size, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (3, 0) _GL_ARG_NONNULL ((3))); _GL_CXXALIAS_RPL (vsnprintf, int, (char *str, size_t size, const char *format, va_list args)); # else # if !@HAVE_DECL_VSNPRINTF@ _GL_FUNCDECL_SYS (vsnprintf, int, (char *str, size_t size, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (3, 0) _GL_ARG_NONNULL ((3))); # endif _GL_CXXALIAS_SYS (vsnprintf, int, (char *str, size_t size, const char *format, va_list args)); # endif _GL_CXXALIASWARN (vsnprintf); #elif defined GNULIB_POSIXCHECK # undef vsnprintf # if HAVE_RAW_DECL_VSNPRINTF _GL_WARN_ON_USE (vsnprintf, "vsnprintf is unportable - " "use gnulib module vsnprintf for portability"); # endif #endif #if @GNULIB_VSPRINTF_POSIX@ # if @REPLACE_VSPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define vsprintf rpl_vsprintf # endif _GL_FUNCDECL_RPL (vsprintf, int, (char *str, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (vsprintf, int, (char *str, const char *format, va_list args)); # else /* Need to cast, because on Solaris, the third parameter is __va_list args and GCC's fixincludes did not change this to __gnuc_va_list. */ _GL_CXXALIAS_SYS_CAST (vsprintf, int, (char *str, const char *format, va_list args)); # endif _GL_CXXALIASWARN (vsprintf); #elif defined GNULIB_POSIXCHECK # undef vsprintf /* Assume vsprintf is always declared. */ _GL_WARN_ON_USE (vsprintf, "vsprintf is not always POSIX compliant - " "use gnulib module vsprintf-posix for portable " "POSIX compliance"); #endif #endif /* _@GUARD_PREFIX@_STDIO_H */ #endif /* _@GUARD_PREFIX@_STDIO_H */ #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/stdint.in.h0000644000175000017500000005261113004436754016467 00000000000000/* Copyright (C) 2001-2002, 2004-2016 Free Software Foundation, Inc. Written by Paul Eggert, Bruno Haible, Sam Steingold, Peter Burwood. This file is part of gnulib. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* * ISO C 99 for platforms that lack it. * */ #ifndef _@GUARD_PREFIX@_STDINT_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* When including a system file that in turn includes , use the system , not our substitute. This avoids problems with (for example) VMS, whose includes . */ #define _GL_JUST_INCLUDE_SYSTEM_INTTYPES_H /* On Android (Bionic libc), includes this file before having defined 'time_t'. Therefore in this case avoid including other system header files; just include the system's . Ideally we should test __BIONIC__ here, but it is only defined after has been included; hence test __ANDROID__ instead. */ #if defined __ANDROID__ && defined _GL_INCLUDING_SYS_TYPES_H # @INCLUDE_NEXT@ @NEXT_STDINT_H@ #else /* Get those types that are already defined in other system include files, so that we can "#define int8_t signed char" below without worrying about a later system include file containing a "typedef signed char int8_t;" that will get messed up by our macro. Our macros should all be consistent with the system versions, except for the "fast" types and macros, which we recommend against using in public interfaces due to compiler differences. */ #if @HAVE_STDINT_H@ # if defined __sgi && ! defined __c99 /* Bypass IRIX's if in C89 mode, since it merely annoys users with "This header file is to be used only for c99 mode compilations" diagnostics. */ # define __STDINT_H__ # endif /* Some pre-C++11 implementations need this. */ # ifdef __cplusplus # ifndef __STDC_CONSTANT_MACROS # define __STDC_CONSTANT_MACROS 1 # endif # ifndef __STDC_LIMIT_MACROS # define __STDC_LIMIT_MACROS 1 # endif # endif /* Other systems may have an incomplete or buggy . Include it before , since any "#include " in would reinclude us, skipping our contents because _@GUARD_PREFIX@_STDINT_H is defined. The include_next requires a split double-inclusion guard. */ # @INCLUDE_NEXT@ @NEXT_STDINT_H@ #endif #if ! defined _@GUARD_PREFIX@_STDINT_H && ! defined _GL_JUST_INCLUDE_SYSTEM_STDINT_H #define _@GUARD_PREFIX@_STDINT_H /* Get SCHAR_MIN, SCHAR_MAX, UCHAR_MAX, INT_MIN, INT_MAX, LONG_MIN, LONG_MAX, ULONG_MAX, _GL_INTEGER_WIDTH. */ #include #if ! @HAVE_C99_STDINT_H@ /* defines some of the stdint.h types as well, on glibc, IRIX 6.5, and OpenBSD 3.8 (via ). AIX 5.2 isn't needed and causes troubles. Mac OS X 10.4.6 includes (which is us), but relies on the system definitions, so include after @NEXT_STDINT_H@. */ # if @HAVE_SYS_TYPES_H@ && ! defined _AIX # include # endif # if @HAVE_INTTYPES_H@ /* In OpenBSD 3.8, includes , which defines int{8,16,32,64}_t, uint{8,16,32,64}_t and __BIT_TYPES_DEFINED__. also defines intptr_t and uintptr_t. */ # include # elif @HAVE_SYS_INTTYPES_H@ /* Solaris 7 has the types except the *_fast*_t types, and the macros except for *_FAST*_*, INTPTR_MIN, PTRDIFF_MIN, PTRDIFF_MAX. */ # include # endif # if @HAVE_SYS_BITYPES_H@ && ! defined __BIT_TYPES_DEFINED__ /* Linux libc4 >= 4.6.7 and libc5 have a that defines int{8,16,32,64}_t and __BIT_TYPES_DEFINED__. In libc5 >= 5.2.2 it is included by . */ # include # endif # undef _GL_JUST_INCLUDE_SYSTEM_INTTYPES_H /* Minimum and maximum values for an integer type under the usual assumption. Return an unspecified value if BITS == 0, adding a check to pacify picky compilers. */ # define _STDINT_MIN(signed, bits, zero) \ ((signed) ? ~ _STDINT_MAX (signed, bits, zero) : (zero)) # define _STDINT_MAX(signed, bits, zero) \ (((((zero) + 1) << ((bits) ? (bits) - 1 - (signed) : 0)) - 1) * 2 + 1) #if !GNULIB_defined_stdint_types /* 7.18.1.1. Exact-width integer types */ /* Here we assume a standard architecture where the hardware integer types have 8, 16, 32, optionally 64 bits. */ # undef int8_t # undef uint8_t typedef signed char gl_int8_t; typedef unsigned char gl_uint8_t; # define int8_t gl_int8_t # define uint8_t gl_uint8_t # undef int16_t # undef uint16_t typedef short int gl_int16_t; typedef unsigned short int gl_uint16_t; # define int16_t gl_int16_t # define uint16_t gl_uint16_t # undef int32_t # undef uint32_t typedef int gl_int32_t; typedef unsigned int gl_uint32_t; # define int32_t gl_int32_t # define uint32_t gl_uint32_t /* If the system defines INT64_MAX, assume int64_t works. That way, if the underlying platform defines int64_t to be a 64-bit long long int, the code below won't mistakenly define it to be a 64-bit long int, which would mess up C++ name mangling. We must use #ifdef rather than #if, to avoid an error with HP-UX 10.20 cc. */ # ifdef INT64_MAX # define GL_INT64_T # else /* Do not undefine int64_t if gnulib is not being used with 64-bit types, since otherwise it breaks platforms like Tandem/NSK. */ # if LONG_MAX >> 31 >> 31 == 1 # undef int64_t typedef long int gl_int64_t; # define int64_t gl_int64_t # define GL_INT64_T # elif defined _MSC_VER # undef int64_t typedef __int64 gl_int64_t; # define int64_t gl_int64_t # define GL_INT64_T # elif @HAVE_LONG_LONG_INT@ # undef int64_t typedef long long int gl_int64_t; # define int64_t gl_int64_t # define GL_INT64_T # endif # endif # ifdef UINT64_MAX # define GL_UINT64_T # else # if ULONG_MAX >> 31 >> 31 >> 1 == 1 # undef uint64_t typedef unsigned long int gl_uint64_t; # define uint64_t gl_uint64_t # define GL_UINT64_T # elif defined _MSC_VER # undef uint64_t typedef unsigned __int64 gl_uint64_t; # define uint64_t gl_uint64_t # define GL_UINT64_T # elif @HAVE_UNSIGNED_LONG_LONG_INT@ # undef uint64_t typedef unsigned long long int gl_uint64_t; # define uint64_t gl_uint64_t # define GL_UINT64_T # endif # endif /* Avoid collision with Solaris 2.5.1 etc. */ # define _UINT8_T # define _UINT32_T # define _UINT64_T /* 7.18.1.2. Minimum-width integer types */ /* Here we assume a standard architecture where the hardware integer types have 8, 16, 32, optionally 64 bits. Therefore the leastN_t types are the same as the corresponding N_t types. */ # undef int_least8_t # undef uint_least8_t # undef int_least16_t # undef uint_least16_t # undef int_least32_t # undef uint_least32_t # undef int_least64_t # undef uint_least64_t # define int_least8_t int8_t # define uint_least8_t uint8_t # define int_least16_t int16_t # define uint_least16_t uint16_t # define int_least32_t int32_t # define uint_least32_t uint32_t # ifdef GL_INT64_T # define int_least64_t int64_t # endif # ifdef GL_UINT64_T # define uint_least64_t uint64_t # endif /* 7.18.1.3. Fastest minimum-width integer types */ /* Note: Other substitutes may define these types differently. It is not recommended to use these types in public header files. */ /* Here we assume a standard architecture where the hardware integer types have 8, 16, 32, optionally 64 bits. Therefore the fastN_t types are taken from the same list of types. The following code normally uses types consistent with glibc, as that lessens the chance of incompatibility with older GNU hosts. */ # undef int_fast8_t # undef uint_fast8_t # undef int_fast16_t # undef uint_fast16_t # undef int_fast32_t # undef uint_fast32_t # undef int_fast64_t # undef uint_fast64_t typedef signed char gl_int_fast8_t; typedef unsigned char gl_uint_fast8_t; # ifdef __sun /* Define types compatible with SunOS 5.10, so that code compiled under earlier SunOS versions works with code compiled under SunOS 5.10. */ typedef int gl_int_fast32_t; typedef unsigned int gl_uint_fast32_t; # else typedef long int gl_int_fast32_t; typedef unsigned long int gl_uint_fast32_t; # endif typedef gl_int_fast32_t gl_int_fast16_t; typedef gl_uint_fast32_t gl_uint_fast16_t; # define int_fast8_t gl_int_fast8_t # define uint_fast8_t gl_uint_fast8_t # define int_fast16_t gl_int_fast16_t # define uint_fast16_t gl_uint_fast16_t # define int_fast32_t gl_int_fast32_t # define uint_fast32_t gl_uint_fast32_t # ifdef GL_INT64_T # define int_fast64_t int64_t # endif # ifdef GL_UINT64_T # define uint_fast64_t uint64_t # endif /* 7.18.1.4. Integer types capable of holding object pointers */ /* kLIBC's stdint.h defines _INTPTR_T_DECLARED and needs its own definitions of intptr_t and uintptr_t (which use int and unsigned) to avoid clashes with declarations of system functions like sbrk. */ # ifndef _INTPTR_T_DECLARED # undef intptr_t # undef uintptr_t typedef long int gl_intptr_t; typedef unsigned long int gl_uintptr_t; # define intptr_t gl_intptr_t # define uintptr_t gl_uintptr_t # endif /* 7.18.1.5. Greatest-width integer types */ /* Note: These types are compiler dependent. It may be unwise to use them in public header files. */ /* If the system defines INTMAX_MAX, assume that intmax_t works, and similarly for UINTMAX_MAX and uintmax_t. This avoids problems with assuming one type where another is used by the system. */ # ifndef INTMAX_MAX # undef INTMAX_C # undef intmax_t # if @HAVE_LONG_LONG_INT@ && LONG_MAX >> 30 == 1 typedef long long int gl_intmax_t; # define intmax_t gl_intmax_t # elif defined GL_INT64_T # define intmax_t int64_t # else typedef long int gl_intmax_t; # define intmax_t gl_intmax_t # endif # endif # ifndef UINTMAX_MAX # undef UINTMAX_C # undef uintmax_t # if @HAVE_UNSIGNED_LONG_LONG_INT@ && ULONG_MAX >> 31 == 1 typedef unsigned long long int gl_uintmax_t; # define uintmax_t gl_uintmax_t # elif defined GL_UINT64_T # define uintmax_t uint64_t # else typedef unsigned long int gl_uintmax_t; # define uintmax_t gl_uintmax_t # endif # endif /* Verify that intmax_t and uintmax_t have the same size. Too much code breaks if this is not the case. If this check fails, the reason is likely to be found in the autoconf macros. */ typedef int _verify_intmax_size[sizeof (intmax_t) == sizeof (uintmax_t) ? 1 : -1]; # define GNULIB_defined_stdint_types 1 # endif /* !GNULIB_defined_stdint_types */ /* 7.18.2. Limits of specified-width integer types */ /* 7.18.2.1. Limits of exact-width integer types */ /* Here we assume a standard architecture where the hardware integer types have 8, 16, 32, optionally 64 bits. */ # undef INT8_MIN # undef INT8_MAX # undef UINT8_MAX # define INT8_MIN (~ INT8_MAX) # define INT8_MAX 127 # define UINT8_MAX 255 # undef INT16_MIN # undef INT16_MAX # undef UINT16_MAX # define INT16_MIN (~ INT16_MAX) # define INT16_MAX 32767 # define UINT16_MAX 65535 # undef INT32_MIN # undef INT32_MAX # undef UINT32_MAX # define INT32_MIN (~ INT32_MAX) # define INT32_MAX 2147483647 # define UINT32_MAX 4294967295U # if defined GL_INT64_T && ! defined INT64_MAX /* Prefer (- INTMAX_C (1) << 63) over (~ INT64_MAX) because SunPRO C 5.0 evaluates the latter incorrectly in preprocessor expressions. */ # define INT64_MIN (- INTMAX_C (1) << 63) # define INT64_MAX INTMAX_C (9223372036854775807) # endif # if defined GL_UINT64_T && ! defined UINT64_MAX # define UINT64_MAX UINTMAX_C (18446744073709551615) # endif /* 7.18.2.2. Limits of minimum-width integer types */ /* Here we assume a standard architecture where the hardware integer types have 8, 16, 32, optionally 64 bits. Therefore the leastN_t types are the same as the corresponding N_t types. */ # undef INT_LEAST8_MIN # undef INT_LEAST8_MAX # undef UINT_LEAST8_MAX # define INT_LEAST8_MIN INT8_MIN # define INT_LEAST8_MAX INT8_MAX # define UINT_LEAST8_MAX UINT8_MAX # undef INT_LEAST16_MIN # undef INT_LEAST16_MAX # undef UINT_LEAST16_MAX # define INT_LEAST16_MIN INT16_MIN # define INT_LEAST16_MAX INT16_MAX # define UINT_LEAST16_MAX UINT16_MAX # undef INT_LEAST32_MIN # undef INT_LEAST32_MAX # undef UINT_LEAST32_MAX # define INT_LEAST32_MIN INT32_MIN # define INT_LEAST32_MAX INT32_MAX # define UINT_LEAST32_MAX UINT32_MAX # undef INT_LEAST64_MIN # undef INT_LEAST64_MAX # ifdef GL_INT64_T # define INT_LEAST64_MIN INT64_MIN # define INT_LEAST64_MAX INT64_MAX # endif # undef UINT_LEAST64_MAX # ifdef GL_UINT64_T # define UINT_LEAST64_MAX UINT64_MAX # endif /* 7.18.2.3. Limits of fastest minimum-width integer types */ /* Here we assume a standard architecture where the hardware integer types have 8, 16, 32, optionally 64 bits. Therefore the fastN_t types are taken from the same list of types. */ # undef INT_FAST8_MIN # undef INT_FAST8_MAX # undef UINT_FAST8_MAX # define INT_FAST8_MIN SCHAR_MIN # define INT_FAST8_MAX SCHAR_MAX # define UINT_FAST8_MAX UCHAR_MAX # undef INT_FAST16_MIN # undef INT_FAST16_MAX # undef UINT_FAST16_MAX # define INT_FAST16_MIN INT_FAST32_MIN # define INT_FAST16_MAX INT_FAST32_MAX # define UINT_FAST16_MAX UINT_FAST32_MAX # undef INT_FAST32_MIN # undef INT_FAST32_MAX # undef UINT_FAST32_MAX # ifdef __sun # define INT_FAST32_MIN INT_MIN # define INT_FAST32_MAX INT_MAX # define UINT_FAST32_MAX UINT_MAX # else # define INT_FAST32_MIN LONG_MIN # define INT_FAST32_MAX LONG_MAX # define UINT_FAST32_MAX ULONG_MAX # endif # undef INT_FAST64_MIN # undef INT_FAST64_MAX # ifdef GL_INT64_T # define INT_FAST64_MIN INT64_MIN # define INT_FAST64_MAX INT64_MAX # endif # undef UINT_FAST64_MAX # ifdef GL_UINT64_T # define UINT_FAST64_MAX UINT64_MAX # endif /* 7.18.2.4. Limits of integer types capable of holding object pointers */ # undef INTPTR_MIN # undef INTPTR_MAX # undef UINTPTR_MAX # define INTPTR_MIN LONG_MIN # define INTPTR_MAX LONG_MAX # define UINTPTR_MAX ULONG_MAX /* 7.18.2.5. Limits of greatest-width integer types */ # ifndef INTMAX_MAX # undef INTMAX_MIN # ifdef INT64_MAX # define INTMAX_MIN INT64_MIN # define INTMAX_MAX INT64_MAX # else # define INTMAX_MIN INT32_MIN # define INTMAX_MAX INT32_MAX # endif # endif # ifndef UINTMAX_MAX # ifdef UINT64_MAX # define UINTMAX_MAX UINT64_MAX # else # define UINTMAX_MAX UINT32_MAX # endif # endif /* 7.18.3. Limits of other integer types */ /* ptrdiff_t limits */ # undef PTRDIFF_MIN # undef PTRDIFF_MAX # if @APPLE_UNIVERSAL_BUILD@ # ifdef _LP64 # define PTRDIFF_MIN _STDINT_MIN (1, 64, 0l) # define PTRDIFF_MAX _STDINT_MAX (1, 64, 0l) # else # define PTRDIFF_MIN _STDINT_MIN (1, 32, 0) # define PTRDIFF_MAX _STDINT_MAX (1, 32, 0) # endif # else # define PTRDIFF_MIN \ _STDINT_MIN (1, @BITSIZEOF_PTRDIFF_T@, 0@PTRDIFF_T_SUFFIX@) # define PTRDIFF_MAX \ _STDINT_MAX (1, @BITSIZEOF_PTRDIFF_T@, 0@PTRDIFF_T_SUFFIX@) # endif /* sig_atomic_t limits */ # undef SIG_ATOMIC_MIN # undef SIG_ATOMIC_MAX # define SIG_ATOMIC_MIN \ _STDINT_MIN (@HAVE_SIGNED_SIG_ATOMIC_T@, @BITSIZEOF_SIG_ATOMIC_T@, \ 0@SIG_ATOMIC_T_SUFFIX@) # define SIG_ATOMIC_MAX \ _STDINT_MAX (@HAVE_SIGNED_SIG_ATOMIC_T@, @BITSIZEOF_SIG_ATOMIC_T@, \ 0@SIG_ATOMIC_T_SUFFIX@) /* size_t limit */ # undef SIZE_MAX # if @APPLE_UNIVERSAL_BUILD@ # ifdef _LP64 # define SIZE_MAX _STDINT_MAX (0, 64, 0ul) # else # define SIZE_MAX _STDINT_MAX (0, 32, 0ul) # endif # else # define SIZE_MAX _STDINT_MAX (0, @BITSIZEOF_SIZE_T@, 0@SIZE_T_SUFFIX@) # endif /* wchar_t limits */ /* Get WCHAR_MIN, WCHAR_MAX. This include is not on the top, above, because on OSF/1 4.0 we have a sequence of nested includes -> -> -> , and the latter includes and assumes its types are already defined. */ # if @HAVE_WCHAR_H@ && ! (defined WCHAR_MIN && defined WCHAR_MAX) /* BSD/OS 4.0.1 has a bug: , and must be included before . */ # include # include # include # define _GL_JUST_INCLUDE_SYSTEM_WCHAR_H # include # undef _GL_JUST_INCLUDE_SYSTEM_WCHAR_H # endif # undef WCHAR_MIN # undef WCHAR_MAX # define WCHAR_MIN \ _STDINT_MIN (@HAVE_SIGNED_WCHAR_T@, @BITSIZEOF_WCHAR_T@, 0@WCHAR_T_SUFFIX@) # define WCHAR_MAX \ _STDINT_MAX (@HAVE_SIGNED_WCHAR_T@, @BITSIZEOF_WCHAR_T@, 0@WCHAR_T_SUFFIX@) /* wint_t limits */ # undef WINT_MIN # undef WINT_MAX # define WINT_MIN \ _STDINT_MIN (@HAVE_SIGNED_WINT_T@, @BITSIZEOF_WINT_T@, 0@WINT_T_SUFFIX@) # define WINT_MAX \ _STDINT_MAX (@HAVE_SIGNED_WINT_T@, @BITSIZEOF_WINT_T@, 0@WINT_T_SUFFIX@) /* 7.18.4. Macros for integer constants */ /* 7.18.4.1. Macros for minimum-width integer constants */ /* According to ISO C 99 Technical Corrigendum 1 */ /* Here we assume a standard architecture where the hardware integer types have 8, 16, 32, optionally 64 bits, and int is 32 bits. */ # undef INT8_C # undef UINT8_C # define INT8_C(x) x # define UINT8_C(x) x # undef INT16_C # undef UINT16_C # define INT16_C(x) x # define UINT16_C(x) x # undef INT32_C # undef UINT32_C # define INT32_C(x) x # define UINT32_C(x) x ## U # undef INT64_C # undef UINT64_C # if LONG_MAX >> 31 >> 31 == 1 # define INT64_C(x) x##L # elif defined _MSC_VER # define INT64_C(x) x##i64 # elif @HAVE_LONG_LONG_INT@ # define INT64_C(x) x##LL # endif # if ULONG_MAX >> 31 >> 31 >> 1 == 1 # define UINT64_C(x) x##UL # elif defined _MSC_VER # define UINT64_C(x) x##ui64 # elif @HAVE_UNSIGNED_LONG_LONG_INT@ # define UINT64_C(x) x##ULL # endif /* 7.18.4.2. Macros for greatest-width integer constants */ # ifndef INTMAX_C # if @HAVE_LONG_LONG_INT@ && LONG_MAX >> 30 == 1 # define INTMAX_C(x) x##LL # elif defined GL_INT64_T # define INTMAX_C(x) INT64_C(x) # else # define INTMAX_C(x) x##L # endif # endif # ifndef UINTMAX_C # if @HAVE_UNSIGNED_LONG_LONG_INT@ && ULONG_MAX >> 31 == 1 # define UINTMAX_C(x) x##ULL # elif defined GL_UINT64_T # define UINTMAX_C(x) UINT64_C(x) # else # define UINTMAX_C(x) x##UL # endif # endif #endif /* !@HAVE_C99_STDINT_H@ */ /* Macros specified by ISO/IEC TS 18661-1:2014. */ #if (!defined UINTMAX_WIDTH \ && (defined _GNU_SOURCE || defined __STDC_WANT_IEC_60559_BFP_EXT__)) # ifdef INT8_MAX # define INT8_WIDTH _GL_INTEGER_WIDTH (INT8_MIN, INT8_MAX) # endif # ifdef UINT8_MAX # define UINT8_WIDTH _GL_INTEGER_WIDTH (0, UINT8_MAX) # endif # ifdef INT16_MAX # define INT16_WIDTH _GL_INTEGER_WIDTH (INT16_MIN, INT16_MAX) # endif # ifdef UINT16_MAX # define UINT16_WIDTH _GL_INTEGER_WIDTH (0, UINT16_MAX) # endif # ifdef INT32_MAX # define INT32_WIDTH _GL_INTEGER_WIDTH (INT32_MIN, INT32_MAX) # endif # ifdef UINT32_MAX # define UINT32_WIDTH _GL_INTEGER_WIDTH (0, UINT32_MAX) # endif # ifdef INT64_MAX # define INT64_WIDTH _GL_INTEGER_WIDTH (INT64_MIN, INT64_MAX) # endif # ifdef UINT64_MAX # define UINT64_WIDTH _GL_INTEGER_WIDTH (0, UINT64_MAX) # endif # define INT_LEAST8_WIDTH _GL_INTEGER_WIDTH (INT_LEAST8_MIN, INT_LEAST8_MAX) # define UINT_LEAST8_WIDTH _GL_INTEGER_WIDTH (0, UINT_LEAST8_MAX) # define INT_LEAST16_WIDTH _GL_INTEGER_WIDTH (INT_LEAST16_MIN, INT_LEAST16_MAX) # define UINT_LEAST16_WIDTH _GL_INTEGER_WIDTH (0, UINT_LEAST16_MAX) # define INT_LEAST32_WIDTH _GL_INTEGER_WIDTH (INT_LEAST32_MIN, INT_LEAST32_MAX) # define UINT_LEAST32_WIDTH _GL_INTEGER_WIDTH (0, UINT_LEAST32_MAX) # define INT_LEAST64_WIDTH _GL_INTEGER_WIDTH (INT_LEAST64_MIN, INT_LEAST64_MAX) # define UINT_LEAST64_WIDTH _GL_INTEGER_WIDTH (0, UINT_LEAST64_MAX) # define INT_FAST8_WIDTH _GL_INTEGER_WIDTH (INT_FAST8_MIN, INT_FAST8_MAX) # define UINT_FAST8_WIDTH _GL_INTEGER_WIDTH (0, UINT_FAST8_MAX) # define INT_FAST16_WIDTH _GL_INTEGER_WIDTH (INT_FAST16_MIN, INT_FAST16_MAX) # define UINT_FAST16_WIDTH _GL_INTEGER_WIDTH (0, UINT_FAST16_MAX) # define INT_FAST32_WIDTH _GL_INTEGER_WIDTH (INT_FAST32_MIN, INT_FAST32_MAX) # define UINT_FAST32_WIDTH _GL_INTEGER_WIDTH (0, UINT_FAST32_MAX) # define INT_FAST64_WIDTH _GL_INTEGER_WIDTH (INT_FAST64_MIN, INT_FAST64_MAX) # define UINT_FAST64_WIDTH _GL_INTEGER_WIDTH (0, UINT_FAST64_MAX) # define INTPTR_WIDTH _GL_INTEGER_WIDTH (INTPTR_MIN, INTPTR_MAX) # define UINTPTR_WIDTH _GL_INTEGER_WIDTH (0, UINTPTR_MAX) # define INTMAX_WIDTH _GL_INTEGER_WIDTH (INTMAX_MIN, INTMAX_MAX) # define UINTMAX_WIDTH _GL_INTEGER_WIDTH (0, UINTMAX_MAX) # define PTRDIFF_WIDTH _GL_INTEGER_WIDTH (PTRDIFF_MIN, PTRDIFF_MAX) # define SIZE_WIDTH _GL_INTEGER_WIDTH (0, SIZE_MAX) # define WCHAR_WIDTH _GL_INTEGER_WIDTH (WCHAR_MIN, WCHAR_MAX) # ifdef WINT_MAX # define WINT_WIDTH _GL_INTEGER_WIDTH (WINT_MIN, WINT_MAX) # endif # ifdef SIG_ATOMIC_MAX # define SIG_ATOMIC_WIDTH _GL_INTEGER_WIDTH (SIG_ATOMIC_MIN, SIG_ATOMIC_MAX) # endif #endif /* !WINT_WIDTH && (_GNU_SOURCE || __STDC_WANT_IEC_60559_BFP_EXT__) */ #endif /* _@GUARD_PREFIX@_STDINT_H */ #endif /* !(defined __ANDROID__ && ...) */ #endif /* !defined _@GUARD_PREFIX@_STDINT_H && !defined _GL_JUST_INCLUDE_SYSTEM_STDINT_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/stddef.in.h0000644000175000017500000000726213004436754016435 00000000000000/* A substitute for POSIX 2008 , for platforms that have issues. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Eric Blake. */ /* * POSIX 2008 for platforms that have issues. * */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if defined __need_wchar_t || defined __need_size_t \ || defined __need_ptrdiff_t || defined __need_NULL \ || defined __need_wint_t /* Special invocation convention inside gcc header files. In particular, gcc provides a version of that blindly redefines NULL even when __need_wint_t was defined, even though wint_t is not normally provided by . Hence, we must remember if special invocation has ever been used to obtain wint_t, in which case we need to clean up NULL yet again. */ # if !(defined _@GUARD_PREFIX@_STDDEF_H && defined _GL_STDDEF_WINT_T) # ifdef __need_wint_t # define _GL_STDDEF_WINT_T # endif # @INCLUDE_NEXT@ @NEXT_STDDEF_H@ # endif #else /* Normal invocation convention. */ # ifndef _@GUARD_PREFIX@_STDDEF_H /* The include_next requires a split double-inclusion guard. */ # @INCLUDE_NEXT@ @NEXT_STDDEF_H@ /* On NetBSD 5.0, the definition of NULL lacks proper parentheses. */ # if (@REPLACE_NULL@ \ && (!defined _@GUARD_PREFIX@_STDDEF_H || defined _GL_STDDEF_WINT_T)) # undef NULL # ifdef __cplusplus /* ISO C++ says that the macro NULL must expand to an integer constant expression, hence '((void *) 0)' is not allowed in C++. */ # if __GNUG__ >= 3 /* GNU C++ has a __null macro that behaves like an integer ('int' or 'long') but has the same size as a pointer. Use that, to avoid warnings. */ # define NULL __null # else # define NULL 0L # endif # else # define NULL ((void *) 0) # endif # endif # ifndef _@GUARD_PREFIX@_STDDEF_H # define _@GUARD_PREFIX@_STDDEF_H /* Some platforms lack wchar_t. */ #if !@HAVE_WCHAR_T@ # define wchar_t int #endif /* Some platforms lack max_align_t. The check for _GCC_MAX_ALIGN_T is a hack in case the configure-time test was done with g++ even though we are currently compiling with gcc. */ #if ! (@HAVE_MAX_ALIGN_T@ || defined _GCC_MAX_ALIGN_T) /* On the x86, the maximum storage alignment of double, long, etc. is 4, but GCC's C11 ABI for x86 says that max_align_t has an alignment of 8, and the C11 standard allows this. Work around this problem by using __alignof__ (which returns 8 for double) rather than _Alignof (which returns 4), and align each union member accordingly. */ # ifdef __GNUC__ # define _GL_STDDEF_ALIGNAS(type) \ __attribute__ ((__aligned__ (__alignof__ (type)))) # else # define _GL_STDDEF_ALIGNAS(type) /* */ # endif typedef union { char *__p _GL_STDDEF_ALIGNAS (char *); double __d _GL_STDDEF_ALIGNAS (double); long double __ld _GL_STDDEF_ALIGNAS (long double); long int __i _GL_STDDEF_ALIGNAS (long int); } max_align_t; #endif # endif /* _@GUARD_PREFIX@_STDDEF_H */ # endif /* _@GUARD_PREFIX@_STDDEF_H */ #endif /* __need_XXX */ gnuastro-0.2.33-8a3b/bootstrapped/lib/stdbool.in.h0000644000175000017500000001177213004436754016633 00000000000000/* Copyright (C) 2001-2003, 2006-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2001. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _GL_STDBOOL_H #define _GL_STDBOOL_H /* ISO C 99 for platforms that lack it. */ /* Usage suggestions: Programs that use should be aware of some limitations and standards compliance issues. Standards compliance: - must be #included before 'bool', 'false', 'true' can be used. - You cannot assume that sizeof (bool) == 1. - Programs should not undefine the macros bool, true, and false, as C99 lists that as an "obsolescent feature". Limitations of this substitute, when used in a C89 environment: - must be #included before the '_Bool' type can be used. - You cannot assume that _Bool is a typedef; it might be a macro. - Bit-fields of type 'bool' are not supported. Portable code should use 'unsigned int foo : 1;' rather than 'bool foo : 1;'. - In C99, casts and automatic conversions to '_Bool' or 'bool' are performed in such a way that every nonzero value gets converted to 'true', and zero gets converted to 'false'. This doesn't work with this substitute. With this substitute, only the values 0 and 1 give the expected result when converted to _Bool' or 'bool'. - C99 allows the use of (_Bool)0.0 in constant expressions, but this substitute cannot always provide this property. Also, it is suggested that programs use 'bool' rather than '_Bool'; this isn't required, but 'bool' is more common. */ /* 7.16. Boolean type and values */ /* BeOS already #defines false 0, true 1. We use the same definitions below, but temporarily we have to #undef them. */ #if defined __BEOS__ && !defined __HAIKU__ # include /* defines bool but not _Bool */ # undef false # undef true #endif #ifdef __cplusplus # define _Bool bool # define bool bool #else # if defined __BEOS__ && !defined __HAIKU__ /* A compiler known to have 'bool'. */ /* If the compiler already has both 'bool' and '_Bool', we can assume they are the same types. */ # if !@HAVE__BOOL@ typedef bool _Bool; # endif # else # if !defined __GNUC__ /* If @HAVE__BOOL@: Some HP-UX cc and AIX IBM C compiler versions have compiler bugs when the built-in _Bool type is used. See http://gcc.gnu.org/ml/gcc-patches/2003-12/msg02303.html http://lists.gnu.org/archive/html/bug-coreutils/2005-11/msg00161.html http://lists.gnu.org/archive/html/bug-coreutils/2005-10/msg00086.html Similar bugs are likely with other compilers as well; this file wouldn't be used if was working. So we override the _Bool type. If !@HAVE__BOOL@: Need to define _Bool ourselves. As 'signed char' or as an enum type? Use of a typedef, with SunPRO C, leads to a stupid "warning: _Bool is a keyword in ISO C99". Use of an enum type, with IRIX cc, leads to a stupid "warning(1185): enumerated type mixed with another type". Even the existence of an enum type, without a typedef, "Invalid enumerator. (badenum)" with HP-UX cc on Tru64. The only benefit of the enum, debuggability, is not important with these compilers. So use 'signed char' and no enum. */ # define _Bool signed char # else /* With this compiler, trust the _Bool type if the compiler has it. */ # if !@HAVE__BOOL@ /* For the sake of symbolic names in gdb, define true and false as enum constants, not only as macros. It is tempting to write typedef enum { false = 0, true = 1 } _Bool; so that gdb prints values of type 'bool' symbolically. But then values of type '_Bool' might promote to 'int' or 'unsigned int' (see ISO C 99 6.7.2.2.(4)); however, '_Bool' must promote to 'int' (see ISO C 99 6.3.1.1.(2)). So add a negative value to the enum; this ensures that '_Bool' promotes to 'int'. */ typedef enum { _Bool_must_promote_to_int = -1, false = 0, true = 1 } _Bool; # endif # endif # endif # define bool _Bool #endif /* The other macros must be usable in preprocessor directives. */ #ifdef __cplusplus # define false false # define true true #else # define false 0 # define true 1 #endif #define __bool_true_false_are_defined 1 #endif /* _GL_STDBOOL_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/stdalign.in.h0000644000175000017500000001117113004436754016763 00000000000000/* A substitute for ISO C11 . Copyright 2011-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Paul Eggert and Bruno Haible. */ #ifndef _GL_STDALIGN_H #define _GL_STDALIGN_H /* ISO C11 for platforms that lack it. References: ISO C11 (latest free draft ) sections 6.5.3.4, 6.7.5, 7.15. C++11 (latest free draft ) section 18.10. */ /* alignof (TYPE), also known as _Alignof (TYPE), yields the alignment requirement of a structure member (i.e., slot or field) that is of type TYPE, as an integer constant expression. This differs from GCC's __alignof__ operator, which can yield a better-performing alignment for an object of that type. For example, on x86 with GCC, __alignof__ (double) and __alignof__ (long long) are 8, whereas alignof (double) and alignof (long long) are 4 unless the option '-malign-double' is used. The result cannot be used as a value for an 'enum' constant, if you want to be portable to HP-UX 10.20 cc and AIX 3.2.5 xlc. Include for offsetof. */ #include /* FreeBSD 9.1 , included by and lots of other standard headers, defines conflicting implementations of _Alignas and _Alignof that are no better than ours; override them. */ #undef _Alignas #undef _Alignof /* GCC releases before GCC 4.9 had a bug in _Alignof. See GCC bug 52023 . */ #if (!defined __STDC_VERSION__ || __STDC_VERSION__ < 201112 \ || (defined __GNUC__ && __GNUC__ < 4 + (__GNUC_MINOR__ < 9))) # ifdef __cplusplus # if 201103 <= __cplusplus # define _Alignof(type) alignof (type) # else template struct __alignof_helper { char __a; __t __b; }; # define _Alignof(type) offsetof (__alignof_helper, __b) # endif # else # define _Alignof(type) offsetof (struct { char __a; type __b; }, __b) # endif #endif #if ! (defined __cplusplus && 201103 <= __cplusplus) # define alignof _Alignof #endif #define __alignof_is_defined 1 /* alignas (A), also known as _Alignas (A), aligns a variable or type to the alignment A, where A is an integer constant expression. For example: int alignas (8) foo; struct s { int a; int alignas (8) bar; }; aligns the address of FOO and the offset of BAR to be multiples of 8. A should be a power of two that is at least the type's alignment and at most the implementation's alignment limit. This limit is 2**28 on typical GNUish hosts, and 2**13 on MSVC. To be portable to MSVC through at least version 10.0, A should be an integer constant, as MSVC does not support expressions such as 1 << 3. To be portable to Sun C 5.11, do not align auto variables to anything stricter than their default alignment. The following C11 requirements are not supported here: - If A is zero, alignas has no effect. - alignas can be used multiple times; the strictest one wins. - alignas (TYPE) is equivalent to alignas (alignof (TYPE)). */ #if !defined __STDC_VERSION__ || __STDC_VERSION__ < 201112 # if defined __cplusplus && 201103 <= __cplusplus # define _Alignas(a) alignas (a) # elif ((defined __APPLE__ && defined __MACH__ \ ? 4 < __GNUC__ + (1 <= __GNUC_MINOR__) \ : __GNUC__) \ || 061200 <= __HP_cc || 061200 <= __HP_aCC \ || __ICC || 0x590 <= __SUNPRO_C || 0x0600 <= __xlC__) # define _Alignas(a) __attribute__ ((__aligned__ (a))) # elif 1300 <= _MSC_VER # define _Alignas(a) __declspec (align (a)) # endif #endif #if ((defined _Alignas && ! (defined __cplusplus && 201103 <= __cplusplus)) \ || (defined __STDC_VERSION__ && 201112 <= __STDC_VERSION__)) # define alignas _Alignas #endif #if defined alignas || (defined __cplusplus && 201103 <= __cplusplus) # define __alignas_is_defined 1 #endif #endif /* _GL_STDALIGN_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/regex_internal.h0000644000175000017500000006200613004436754017562 00000000000000/* Extended regular expression matching and search library. Copyright (C) 2002-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Contributed by Isamu Hasegawa . The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ #ifndef _REGEX_INTERNAL_H #define _REGEX_INTERNAL_H 1 #include #include #include #include #include #include #include #include #include #include #include #ifdef _LIBC # include # define lock_define(name) __libc_lock_define (, name) # define lock_init(lock) (__libc_lock_init (lock), 0) # define lock_fini(lock) 0 # define lock_lock(lock) __libc_lock_lock (lock) # define lock_unlock(lock) __libc_lock_unlock (lock) #elif defined GNULIB_LOCK && !defined USE_UNLOCKED_IO # include "glthread/lock.h" /* Use gl_lock_define if empty macro arguments are known to work. Otherwise, fall back on less-portable substitutes. */ # if ((defined __GNUC__ && !defined __STRICT_ANSI__) \ || (defined __STDC_VERSION__ && 199901L <= __STDC_VERSION__)) # define lock_define(name) gl_lock_define (, name) # elif USE_POSIX_THREADS # define lock_define(name) pthread_mutex_t name; # elif USE_PTH_THREADS # define lock_define(name) pth_mutex_t name; # elif USE_SOLARIS_THREADS # define lock_define(name) mutex_t name; # elif USE_WINDOWS_THREADS # define lock_define(name) gl_lock_t name; # else # define lock_define(name) # endif # define lock_init(lock) glthread_lock_init (&(lock)) # define lock_fini(lock) glthread_lock_destroy (&(lock)) # define lock_lock(lock) glthread_lock_lock (&(lock)) # define lock_unlock(lock) glthread_lock_unlock (&(lock)) #elif defined GNULIB_PTHREAD && !defined USE_UNLOCKED_IO # include # define lock_define(name) pthread_mutex_t name; # define lock_init(lock) pthread_mutex_init (&(lock), 0) # define lock_fini(lock) pthread_mutex_destroy (&(lock)) # define lock_lock(lock) pthread_mutex_lock (&(lock)) # define lock_unlock(lock) pthread_mutex_unlock (&(lock)) #else # define lock_define(name) # define lock_init(lock) 0 # define lock_fini(lock) ((void) 0) /* The 'dfa' avoids an "unused variable 'dfa'" warning from GCC. */ # define lock_lock(lock) ((void) dfa) # define lock_unlock(lock) ((void) 0) #endif /* In case that the system doesn't have isblank(). */ #if !defined _LIBC && ! (defined isblank || (HAVE_ISBLANK && HAVE_DECL_ISBLANK)) # define isblank(ch) ((ch) == ' ' || (ch) == '\t') #endif #ifdef _LIBC # ifndef _RE_DEFINE_LOCALE_FUNCTIONS # define _RE_DEFINE_LOCALE_FUNCTIONS 1 # include # include # endif #endif /* This is for other GNU distributions with internationalized messages. */ #if (HAVE_LIBINTL_H && ENABLE_NLS) || defined _LIBC # include # ifdef _LIBC # undef gettext # define gettext(msgid) \ __dcgettext (_libc_intl_domainname, msgid, LC_MESSAGES) # endif #else # define gettext(msgid) (msgid) #endif #ifndef gettext_noop /* This define is so xgettext can find the internationalizable strings. */ # define gettext_noop(String) String #endif #if (defined MB_CUR_MAX && HAVE_WCTYPE_H && HAVE_ISWCTYPE) || _LIBC # define RE_ENABLE_I18N #endif #if __GNUC__ >= 3 # define BE(expr, val) __builtin_expect (expr, val) #else # define BE(expr, val) (expr) #endif /* Number of ASCII characters. */ #define ASCII_CHARS 0x80 /* Number of single byte characters. */ #define SBC_MAX (UCHAR_MAX + 1) #define COLL_ELEM_LEN_MAX 8 /* The character which represents newline. */ #define NEWLINE_CHAR '\n' #define WIDE_NEWLINE_CHAR L'\n' /* Rename to standard API for using out of glibc. */ #ifndef _LIBC # undef __wctype # undef __iswctype # define __wctype wctype # define __iswalnum iswalnum # define __iswctype iswctype # define __towlower towlower # define __towupper towupper # define __btowc btowc # define __mbrtowc mbrtowc # define __wcrtomb wcrtomb # define __regfree regfree # define attribute_hidden #endif /* not _LIBC */ #if __GNUC__ < 3 + (__GNUC_MINOR__ < 1) # define __attribute__(arg) #endif #ifndef SSIZE_MAX # define SSIZE_MAX ((ssize_t) (SIZE_MAX / 2)) #endif /* The type of indexes into strings. This is signed, not size_t, since the API requires indexes to fit in regoff_t anyway, and using signed integers makes the code a bit smaller and presumably faster. The traditional GNU regex implementation uses int for indexes. The POSIX-compatible implementation uses a possibly-wider type. The name 'Idx' is three letters to minimize the hassle of reindenting a lot of regex code that formerly used 'int'. */ typedef regoff_t Idx; #ifdef _REGEX_LARGE_OFFSETS # define IDX_MAX SSIZE_MAX #else # define IDX_MAX INT_MAX #endif /* A hash value, suitable for computing hash tables. */ typedef __re_size_t re_hashval_t; /* An integer used to represent a set of bits. It must be unsigned, and must be at least as wide as unsigned int. */ typedef unsigned long int bitset_word_t; /* All bits set in a bitset_word_t. */ #define BITSET_WORD_MAX ULONG_MAX /* Number of bits in a bitset_word_t. For portability to hosts with padding bits, do not use '(sizeof (bitset_word_t) * CHAR_BIT)'; instead, deduce it directly from BITSET_WORD_MAX. Avoid greater-than-32-bit integers and unconditional shifts by more than 31 bits, as they're not portable. */ #if BITSET_WORD_MAX == 0xffffffffUL # define BITSET_WORD_BITS 32 #elif BITSET_WORD_MAX >> 31 >> 4 == 1 # define BITSET_WORD_BITS 36 #elif BITSET_WORD_MAX >> 31 >> 16 == 1 # define BITSET_WORD_BITS 48 #elif BITSET_WORD_MAX >> 31 >> 28 == 1 # define BITSET_WORD_BITS 60 #elif BITSET_WORD_MAX >> 31 >> 31 >> 1 == 1 # define BITSET_WORD_BITS 64 #elif BITSET_WORD_MAX >> 31 >> 31 >> 9 == 1 # define BITSET_WORD_BITS 72 #elif BITSET_WORD_MAX >> 31 >> 31 >> 31 >> 31 >> 3 == 1 # define BITSET_WORD_BITS 128 #elif BITSET_WORD_MAX >> 31 >> 31 >> 31 >> 31 >> 31 >> 31 >> 31 >> 31 >> 7 == 1 # define BITSET_WORD_BITS 256 #elif BITSET_WORD_MAX >> 31 >> 31 >> 31 >> 31 >> 31 >> 31 >> 31 >> 31 >> 7 > 1 # define BITSET_WORD_BITS 257 /* any value > SBC_MAX will do here */ # if BITSET_WORD_BITS <= SBC_MAX # error "Invalid SBC_MAX" # endif #else # error "Add case for new bitset_word_t size" #endif /* Number of bitset_word_t values in a bitset_t. */ #define BITSET_WORDS ((SBC_MAX + BITSET_WORD_BITS - 1) / BITSET_WORD_BITS) typedef bitset_word_t bitset_t[BITSET_WORDS]; typedef bitset_word_t *re_bitset_ptr_t; typedef const bitset_word_t *re_const_bitset_ptr_t; #define PREV_WORD_CONSTRAINT 0x0001 #define PREV_NOTWORD_CONSTRAINT 0x0002 #define NEXT_WORD_CONSTRAINT 0x0004 #define NEXT_NOTWORD_CONSTRAINT 0x0008 #define PREV_NEWLINE_CONSTRAINT 0x0010 #define NEXT_NEWLINE_CONSTRAINT 0x0020 #define PREV_BEGBUF_CONSTRAINT 0x0040 #define NEXT_ENDBUF_CONSTRAINT 0x0080 #define WORD_DELIM_CONSTRAINT 0x0100 #define NOT_WORD_DELIM_CONSTRAINT 0x0200 typedef enum { INSIDE_WORD = PREV_WORD_CONSTRAINT | NEXT_WORD_CONSTRAINT, WORD_FIRST = PREV_NOTWORD_CONSTRAINT | NEXT_WORD_CONSTRAINT, WORD_LAST = PREV_WORD_CONSTRAINT | NEXT_NOTWORD_CONSTRAINT, INSIDE_NOTWORD = PREV_NOTWORD_CONSTRAINT | NEXT_NOTWORD_CONSTRAINT, LINE_FIRST = PREV_NEWLINE_CONSTRAINT, LINE_LAST = NEXT_NEWLINE_CONSTRAINT, BUF_FIRST = PREV_BEGBUF_CONSTRAINT, BUF_LAST = NEXT_ENDBUF_CONSTRAINT, WORD_DELIM = WORD_DELIM_CONSTRAINT, NOT_WORD_DELIM = NOT_WORD_DELIM_CONSTRAINT } re_context_type; typedef struct { Idx alloc; Idx nelem; Idx *elems; } re_node_set; typedef enum { NON_TYPE = 0, /* Node type, These are used by token, node, tree. */ CHARACTER = 1, END_OF_RE = 2, SIMPLE_BRACKET = 3, OP_BACK_REF = 4, OP_PERIOD = 5, #ifdef RE_ENABLE_I18N COMPLEX_BRACKET = 6, OP_UTF8_PERIOD = 7, #endif /* RE_ENABLE_I18N */ /* We define EPSILON_BIT as a macro so that OP_OPEN_SUBEXP is used when the debugger shows values of this enum type. */ #define EPSILON_BIT 8 OP_OPEN_SUBEXP = EPSILON_BIT | 0, OP_CLOSE_SUBEXP = EPSILON_BIT | 1, OP_ALT = EPSILON_BIT | 2, OP_DUP_ASTERISK = EPSILON_BIT | 3, ANCHOR = EPSILON_BIT | 4, /* Tree type, these are used only by tree. */ CONCAT = 16, SUBEXP = 17, /* Token type, these are used only by token. */ OP_DUP_PLUS = 18, OP_DUP_QUESTION, OP_OPEN_BRACKET, OP_CLOSE_BRACKET, OP_CHARSET_RANGE, OP_OPEN_DUP_NUM, OP_CLOSE_DUP_NUM, OP_NON_MATCH_LIST, OP_OPEN_COLL_ELEM, OP_CLOSE_COLL_ELEM, OP_OPEN_EQUIV_CLASS, OP_CLOSE_EQUIV_CLASS, OP_OPEN_CHAR_CLASS, OP_CLOSE_CHAR_CLASS, OP_WORD, OP_NOTWORD, OP_SPACE, OP_NOTSPACE, BACK_SLASH } re_token_type_t; #ifdef RE_ENABLE_I18N typedef struct { /* Multibyte characters. */ wchar_t *mbchars; /* Collating symbols. */ # ifdef _LIBC int32_t *coll_syms; # endif /* Equivalence classes. */ # ifdef _LIBC int32_t *equiv_classes; # endif /* Range expressions. */ # ifdef _LIBC uint32_t *range_starts; uint32_t *range_ends; # else /* not _LIBC */ wchar_t *range_starts; wchar_t *range_ends; # endif /* not _LIBC */ /* Character classes. */ wctype_t *char_classes; /* If this character set is the non-matching list. */ unsigned int non_match : 1; /* # of multibyte characters. */ Idx nmbchars; /* # of collating symbols. */ Idx ncoll_syms; /* # of equivalence classes. */ Idx nequiv_classes; /* # of range expressions. */ Idx nranges; /* # of character classes. */ Idx nchar_classes; } re_charset_t; #endif /* RE_ENABLE_I18N */ typedef struct { union { unsigned char c; /* for CHARACTER */ re_bitset_ptr_t sbcset; /* for SIMPLE_BRACKET */ #ifdef RE_ENABLE_I18N re_charset_t *mbcset; /* for COMPLEX_BRACKET */ #endif /* RE_ENABLE_I18N */ Idx idx; /* for BACK_REF */ re_context_type ctx_type; /* for ANCHOR */ } opr; #if __GNUC__ >= 2 && !defined __STRICT_ANSI__ re_token_type_t type : 8; #else re_token_type_t type; #endif unsigned int constraint : 10; /* context constraint */ unsigned int duplicated : 1; unsigned int opt_subexp : 1; #ifdef RE_ENABLE_I18N unsigned int accept_mb : 1; /* These 2 bits can be moved into the union if needed (e.g. if running out of bits; move opr.c to opr.c.c and move the flags to opr.c.flags). */ unsigned int mb_partial : 1; #endif unsigned int word_char : 1; } re_token_t; #define IS_EPSILON_NODE(type) ((type) & EPSILON_BIT) struct re_string_t { /* Indicate the raw buffer which is the original string passed as an argument of regexec(), re_search(), etc.. */ const unsigned char *raw_mbs; /* Store the multibyte string. In case of "case insensitive mode" like REG_ICASE, upper cases of the string are stored, otherwise MBS points the same address that RAW_MBS points. */ unsigned char *mbs; #ifdef RE_ENABLE_I18N /* Store the wide character string which is corresponding to MBS. */ wint_t *wcs; Idx *offsets; mbstate_t cur_state; #endif /* Index in RAW_MBS. Each character mbs[i] corresponds to raw_mbs[raw_mbs_idx + i]. */ Idx raw_mbs_idx; /* The length of the valid characters in the buffers. */ Idx valid_len; /* The corresponding number of bytes in raw_mbs array. */ Idx valid_raw_len; /* The length of the buffers MBS and WCS. */ Idx bufs_len; /* The index in MBS, which is updated by re_string_fetch_byte. */ Idx cur_idx; /* length of RAW_MBS array. */ Idx raw_len; /* This is RAW_LEN - RAW_MBS_IDX + VALID_LEN - VALID_RAW_LEN. */ Idx len; /* End of the buffer may be shorter than its length in the cases such as re_match_2, re_search_2. Then, we use STOP for end of the buffer instead of LEN. */ Idx raw_stop; /* This is RAW_STOP - RAW_MBS_IDX adjusted through OFFSETS. */ Idx stop; /* The context of mbs[0]. We store the context independently, since the context of mbs[0] may be different from raw_mbs[0], which is the beginning of the input string. */ unsigned int tip_context; /* The translation passed as a part of an argument of re_compile_pattern. */ RE_TRANSLATE_TYPE trans; /* Copy of re_dfa_t's word_char. */ re_const_bitset_ptr_t word_char; /* true if REG_ICASE. */ unsigned char icase; unsigned char is_utf8; unsigned char map_notascii; unsigned char mbs_allocated; unsigned char offsets_needed; unsigned char newline_anchor; unsigned char word_ops_used; int mb_cur_max; }; typedef struct re_string_t re_string_t; struct re_dfa_t; typedef struct re_dfa_t re_dfa_t; #ifndef _LIBC # define internal_function # define IS_IN(libc) false #endif static reg_errcode_t re_string_realloc_buffers (re_string_t *pstr, Idx new_buf_len) internal_function; #ifdef RE_ENABLE_I18N static void build_wcs_buffer (re_string_t *pstr) internal_function; static reg_errcode_t build_wcs_upper_buffer (re_string_t *pstr) internal_function; #endif /* RE_ENABLE_I18N */ static void build_upper_buffer (re_string_t *pstr) internal_function; static void re_string_translate_buffer (re_string_t *pstr) internal_function; static unsigned int re_string_context_at (const re_string_t *input, Idx idx, int eflags) internal_function __attribute__ ((pure)); #define re_string_peek_byte(pstr, offset) \ ((pstr)->mbs[(pstr)->cur_idx + offset]) #define re_string_fetch_byte(pstr) \ ((pstr)->mbs[(pstr)->cur_idx++]) #define re_string_first_byte(pstr, idx) \ ((idx) == (pstr)->valid_len || (pstr)->wcs[idx] != WEOF) #define re_string_is_single_byte_char(pstr, idx) \ ((pstr)->wcs[idx] != WEOF && ((pstr)->valid_len == (idx) + 1 \ || (pstr)->wcs[(idx) + 1] != WEOF)) #define re_string_eoi(pstr) ((pstr)->stop <= (pstr)->cur_idx) #define re_string_cur_idx(pstr) ((pstr)->cur_idx) #define re_string_get_buffer(pstr) ((pstr)->mbs) #define re_string_length(pstr) ((pstr)->len) #define re_string_byte_at(pstr,idx) ((pstr)->mbs[idx]) #define re_string_skip_bytes(pstr,idx) ((pstr)->cur_idx += (idx)) #define re_string_set_index(pstr,idx) ((pstr)->cur_idx = (idx)) #if defined _LIBC || HAVE_ALLOCA # include #endif #ifndef _LIBC # if HAVE_ALLOCA /* The OS usually guarantees only one guard page at the bottom of the stack, and a page size can be as small as 4096 bytes. So we cannot safely allocate anything larger than 4096 bytes. Also care for the possibility of a few compiler-allocated temporary stack slots. */ # define __libc_use_alloca(n) ((n) < 4032) # else /* alloca is implemented with malloc, so just use malloc. */ # define __libc_use_alloca(n) 0 # undef alloca # define alloca(n) malloc (n) # endif #endif #ifdef _LIBC # define MALLOC_0_IS_NONNULL 1 #elif !defined MALLOC_0_IS_NONNULL # define MALLOC_0_IS_NONNULL 0 #endif #ifndef MAX # define MAX(a,b) ((a) < (b) ? (b) : (a)) #endif #ifndef MIN # define MIN(a,b) ((a) < (b) ? (a) : (b)) #endif #define re_malloc(t,n) ((t *) malloc ((n) * sizeof (t))) #define re_realloc(p,t,n) ((t *) realloc (p, (n) * sizeof (t))) #define re_free(p) free (p) struct bin_tree_t { struct bin_tree_t *parent; struct bin_tree_t *left; struct bin_tree_t *right; struct bin_tree_t *first; struct bin_tree_t *next; re_token_t token; /* 'node_idx' is the index in dfa->nodes, if 'type' == 0. Otherwise 'type' indicate the type of this node. */ Idx node_idx; }; typedef struct bin_tree_t bin_tree_t; #define BIN_TREE_STORAGE_SIZE \ ((1024 - sizeof (void *)) / sizeof (bin_tree_t)) struct bin_tree_storage_t { struct bin_tree_storage_t *next; bin_tree_t data[BIN_TREE_STORAGE_SIZE]; }; typedef struct bin_tree_storage_t bin_tree_storage_t; #define CONTEXT_WORD 1 #define CONTEXT_NEWLINE (CONTEXT_WORD << 1) #define CONTEXT_BEGBUF (CONTEXT_NEWLINE << 1) #define CONTEXT_ENDBUF (CONTEXT_BEGBUF << 1) #define IS_WORD_CONTEXT(c) ((c) & CONTEXT_WORD) #define IS_NEWLINE_CONTEXT(c) ((c) & CONTEXT_NEWLINE) #define IS_BEGBUF_CONTEXT(c) ((c) & CONTEXT_BEGBUF) #define IS_ENDBUF_CONTEXT(c) ((c) & CONTEXT_ENDBUF) #define IS_ORDINARY_CONTEXT(c) ((c) == 0) #define IS_WORD_CHAR(ch) (isalnum (ch) || (ch) == '_') #define IS_NEWLINE(ch) ((ch) == NEWLINE_CHAR) #define IS_WIDE_WORD_CHAR(ch) (__iswalnum (ch) || (ch) == L'_') #define IS_WIDE_NEWLINE(ch) ((ch) == WIDE_NEWLINE_CHAR) #define NOT_SATISFY_PREV_CONSTRAINT(constraint,context) \ ((((constraint) & PREV_WORD_CONSTRAINT) && !IS_WORD_CONTEXT (context)) \ || ((constraint & PREV_NOTWORD_CONSTRAINT) && IS_WORD_CONTEXT (context)) \ || ((constraint & PREV_NEWLINE_CONSTRAINT) && !IS_NEWLINE_CONTEXT (context))\ || ((constraint & PREV_BEGBUF_CONSTRAINT) && !IS_BEGBUF_CONTEXT (context))) #define NOT_SATISFY_NEXT_CONSTRAINT(constraint,context) \ ((((constraint) & NEXT_WORD_CONSTRAINT) && !IS_WORD_CONTEXT (context)) \ || (((constraint) & NEXT_NOTWORD_CONSTRAINT) && IS_WORD_CONTEXT (context)) \ || (((constraint) & NEXT_NEWLINE_CONSTRAINT) && !IS_NEWLINE_CONTEXT (context)) \ || (((constraint) & NEXT_ENDBUF_CONSTRAINT) && !IS_ENDBUF_CONTEXT (context))) struct re_dfastate_t { re_hashval_t hash; re_node_set nodes; re_node_set non_eps_nodes; re_node_set inveclosure; re_node_set *entrance_nodes; struct re_dfastate_t **trtable, **word_trtable; unsigned int context : 4; unsigned int halt : 1; /* If this state can accept "multi byte". Note that we refer to multibyte characters, and multi character collating elements as "multi byte". */ unsigned int accept_mb : 1; /* If this state has backreference node(s). */ unsigned int has_backref : 1; unsigned int has_constraint : 1; }; typedef struct re_dfastate_t re_dfastate_t; struct re_state_table_entry { Idx num; Idx alloc; re_dfastate_t **array; }; /* Array type used in re_sub_match_last_t and re_sub_match_top_t. */ typedef struct { Idx next_idx; Idx alloc; re_dfastate_t **array; } state_array_t; /* Store information about the node NODE whose type is OP_CLOSE_SUBEXP. */ typedef struct { Idx node; Idx str_idx; /* The position NODE match at. */ state_array_t path; } re_sub_match_last_t; /* Store information about the node NODE whose type is OP_OPEN_SUBEXP. And information about the node, whose type is OP_CLOSE_SUBEXP, corresponding to NODE is stored in LASTS. */ typedef struct { Idx str_idx; Idx node; state_array_t *path; Idx alasts; /* Allocation size of LASTS. */ Idx nlasts; /* The number of LASTS. */ re_sub_match_last_t **lasts; } re_sub_match_top_t; struct re_backref_cache_entry { Idx node; Idx str_idx; Idx subexp_from; Idx subexp_to; char more; char unused; unsigned short int eps_reachable_subexps_map; }; typedef struct { /* The string object corresponding to the input string. */ re_string_t input; #if defined _LIBC || (defined __STDC_VERSION__ && __STDC_VERSION__ >= 199901L) const re_dfa_t *const dfa; #else const re_dfa_t *dfa; #endif /* EFLAGS of the argument of regexec. */ int eflags; /* Where the matching ends. */ Idx match_last; Idx last_node; /* The state log used by the matcher. */ re_dfastate_t **state_log; Idx state_log_top; /* Back reference cache. */ Idx nbkref_ents; Idx abkref_ents; struct re_backref_cache_entry *bkref_ents; int max_mb_elem_len; Idx nsub_tops; Idx asub_tops; re_sub_match_top_t **sub_tops; } re_match_context_t; typedef struct { re_dfastate_t **sifted_states; re_dfastate_t **limited_states; Idx last_node; Idx last_str_idx; re_node_set limits; } re_sift_context_t; struct re_fail_stack_ent_t { Idx idx; Idx node; regmatch_t *regs; re_node_set eps_via_nodes; }; struct re_fail_stack_t { Idx num; Idx alloc; struct re_fail_stack_ent_t *stack; }; struct re_dfa_t { re_token_t *nodes; size_t nodes_alloc; size_t nodes_len; Idx *nexts; Idx *org_indices; re_node_set *edests; re_node_set *eclosures; re_node_set *inveclosures; struct re_state_table_entry *state_table; re_dfastate_t *init_state; re_dfastate_t *init_state_word; re_dfastate_t *init_state_nl; re_dfastate_t *init_state_begbuf; bin_tree_t *str_tree; bin_tree_storage_t *str_tree_storage; re_bitset_ptr_t sb_char; int str_tree_storage_idx; /* number of subexpressions 're_nsub' is in regex_t. */ re_hashval_t state_hash_mask; Idx init_node; Idx nbackref; /* The number of backreference in this dfa. */ /* Bitmap expressing which backreference is used. */ bitset_word_t used_bkref_map; bitset_word_t completed_bkref_map; unsigned int has_plural_match : 1; /* If this dfa has "multibyte node", which is a backreference or a node which can accept multibyte character or multi character collating element. */ unsigned int has_mb_node : 1; unsigned int is_utf8 : 1; unsigned int map_notascii : 1; unsigned int word_ops_used : 1; int mb_cur_max; bitset_t word_char; reg_syntax_t syntax; Idx *subexp_map; #ifdef DEBUG char* re_str; #endif lock_define (lock) }; #define re_node_set_init_empty(set) memset (set, '\0', sizeof (re_node_set)) #define re_node_set_remove(set,id) \ (re_node_set_remove_at (set, re_node_set_contains (set, id) - 1)) #define re_node_set_empty(p) ((p)->nelem = 0) #define re_node_set_free(set) re_free ((set)->elems) typedef enum { SB_CHAR, MB_CHAR, EQUIV_CLASS, COLL_SYM, CHAR_CLASS } bracket_elem_type; typedef struct { bracket_elem_type type; union { unsigned char ch; unsigned char *name; wchar_t wch; } opr; } bracket_elem_t; /* Functions for bitset_t operation. */ static void bitset_set (bitset_t set, Idx i) { set[i / BITSET_WORD_BITS] |= (bitset_word_t) 1 << i % BITSET_WORD_BITS; } static void bitset_clear (bitset_t set, Idx i) { set[i / BITSET_WORD_BITS] &= ~ ((bitset_word_t) 1 << i % BITSET_WORD_BITS); } static bool bitset_contain (const bitset_t set, Idx i) { return (set[i / BITSET_WORD_BITS] >> i % BITSET_WORD_BITS) & 1; } static void bitset_empty (bitset_t set) { memset (set, '\0', sizeof (bitset_t)); } static void bitset_set_all (bitset_t set) { memset (set, -1, sizeof (bitset_word_t) * (SBC_MAX / BITSET_WORD_BITS)); if (SBC_MAX % BITSET_WORD_BITS != 0) set[BITSET_WORDS - 1] = ((bitset_word_t) 1 << SBC_MAX % BITSET_WORD_BITS) - 1; } static void bitset_copy (bitset_t dest, const bitset_t src) { memcpy (dest, src, sizeof (bitset_t)); } static void __attribute__ ((unused)) bitset_not (bitset_t set) { int bitset_i; for (bitset_i = 0; bitset_i < SBC_MAX / BITSET_WORD_BITS; ++bitset_i) set[bitset_i] = ~set[bitset_i]; if (SBC_MAX % BITSET_WORD_BITS != 0) set[BITSET_WORDS - 1] = ((((bitset_word_t) 1 << SBC_MAX % BITSET_WORD_BITS) - 1) & ~set[BITSET_WORDS - 1]); } static void __attribute__ ((unused)) bitset_merge (bitset_t dest, const bitset_t src) { int bitset_i; for (bitset_i = 0; bitset_i < BITSET_WORDS; ++bitset_i) dest[bitset_i] |= src[bitset_i]; } static void __attribute__ ((unused)) bitset_mask (bitset_t dest, const bitset_t src) { int bitset_i; for (bitset_i = 0; bitset_i < BITSET_WORDS; ++bitset_i) dest[bitset_i] &= src[bitset_i]; } #ifdef RE_ENABLE_I18N /* Functions for re_string. */ static int internal_function __attribute__ ((pure, unused)) re_string_char_size_at (const re_string_t *pstr, Idx idx) { int byte_idx; if (pstr->mb_cur_max == 1) return 1; for (byte_idx = 1; idx + byte_idx < pstr->valid_len; ++byte_idx) if (pstr->wcs[idx + byte_idx] != WEOF) break; return byte_idx; } static wint_t internal_function __attribute__ ((pure, unused)) re_string_wchar_at (const re_string_t *pstr, Idx idx) { if (pstr->mb_cur_max == 1) return (wint_t) pstr->mbs[idx]; return (wint_t) pstr->wcs[idx]; } # ifdef _LIBC # include # endif static int internal_function __attribute__ ((pure, unused)) re_string_elem_size_at (const re_string_t *pstr, Idx idx) { # ifdef _LIBC const unsigned char *p, *extra; const int32_t *table, *indirect; uint_fast32_t nrules = _NL_CURRENT_WORD (LC_COLLATE, _NL_COLLATE_NRULES); if (nrules != 0) { table = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_TABLEMB); extra = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_EXTRAMB); indirect = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_INDIRECTMB); p = pstr->mbs + idx; findidx (table, indirect, extra, &p, pstr->len - idx); return p - pstr->mbs - idx; } else # endif /* _LIBC */ return 1; } #endif /* RE_ENABLE_I18N */ #ifndef __GNUC_PREREQ # if defined __GNUC__ && defined __GNUC_MINOR__ # define __GNUC_PREREQ(maj, min) \ ((__GNUC__ << 16) + __GNUC_MINOR__ >= ((maj) << 16) + (min)) # else # define __GNUC_PREREQ(maj, min) 0 # endif #endif #if __GNUC_PREREQ (3,4) # undef __attribute_warn_unused_result__ # define __attribute_warn_unused_result__ \ __attribute__ ((__warn_unused_result__)) #else # define __attribute_warn_unused_result__ /* empty */ #endif #endif /* _REGEX_INTERNAL_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/regex.h0000644000175000017500000006013413004436754015666 00000000000000/* Definitions for data structures and routines for the regular expression library. Copyright (C) 1985, 1989-1993, 1995-1998, 2000-2003, 2005-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ #ifndef _REGEX_H #define _REGEX_H 1 #include /* Allow the use in C++ code. */ #ifdef __cplusplus extern "C" { #endif /* Define __USE_GNU to declare GNU extensions that violate the POSIX name space rules. */ #ifdef _GNU_SOURCE # define __USE_GNU 1 #endif #ifdef _REGEX_LARGE_OFFSETS /* Use types and values that are wide enough to represent signed and unsigned byte offsets in memory. This currently works only when the regex code is used outside of the GNU C library; it is not yet supported within glibc itself, and glibc users should not define _REGEX_LARGE_OFFSETS. */ /* The type of object sizes. */ typedef size_t __re_size_t; /* The type of object sizes, in places where the traditional code uses unsigned long int. */ typedef size_t __re_long_size_t; #else /* The traditional GNU regex implementation mishandles strings longer than INT_MAX. */ typedef unsigned int __re_size_t; typedef unsigned long int __re_long_size_t; #endif /* The following two types have to be signed and unsigned integer type wide enough to hold a value of a pointer. For most ANSI compilers ptrdiff_t and size_t should be likely OK. Still size of these two types is 2 for Microsoft C. Ugh... */ typedef long int s_reg_t; typedef unsigned long int active_reg_t; /* The following bits are used to determine the regexp syntax we recognize. The set/not-set meanings are chosen so that Emacs syntax remains the value 0. The bits are given in alphabetical order, and the definitions shifted by one from the previous bit; thus, when we add or remove a bit, only one other definition need change. */ typedef unsigned long int reg_syntax_t; #ifdef __USE_GNU /* If this bit is not set, then \ inside a bracket expression is literal. If set, then such a \ quotes the following character. */ # define RE_BACKSLASH_ESCAPE_IN_LISTS ((unsigned long int) 1) /* If this bit is not set, then + and ? are operators, and \+ and \? are literals. If set, then \+ and \? are operators and + and ? are literals. */ # define RE_BK_PLUS_QM (RE_BACKSLASH_ESCAPE_IN_LISTS << 1) /* If this bit is set, then character classes are supported. They are: [:alpha:], [:upper:], [:lower:], [:digit:], [:alnum:], [:xdigit:], [:space:], [:print:], [:punct:], [:graph:], and [:cntrl:]. If not set, then character classes are not supported. */ # define RE_CHAR_CLASSES (RE_BK_PLUS_QM << 1) /* If this bit is set, then ^ and $ are always anchors (outside bracket expressions, of course). If this bit is not set, then it depends: ^ is an anchor if it is at the beginning of a regular expression or after an open-group or an alternation operator; $ is an anchor if it is at the end of a regular expression, or before a close-group or an alternation operator. This bit could be (re)combined with RE_CONTEXT_INDEP_OPS, because POSIX draft 11.2 says that * etc. in leading positions is undefined. We already implemented a previous draft which made those constructs invalid, though, so we haven't changed the code back. */ # define RE_CONTEXT_INDEP_ANCHORS (RE_CHAR_CLASSES << 1) /* If this bit is set, then special characters are always special regardless of where they are in the pattern. If this bit is not set, then special characters are special only in some contexts; otherwise they are ordinary. Specifically, * + ? and intervals are only special when not after the beginning, open-group, or alternation operator. */ # define RE_CONTEXT_INDEP_OPS (RE_CONTEXT_INDEP_ANCHORS << 1) /* If this bit is set, then *, +, ?, and { cannot be first in an re or immediately after an alternation or begin-group operator. */ # define RE_CONTEXT_INVALID_OPS (RE_CONTEXT_INDEP_OPS << 1) /* If this bit is set, then . matches newline. If not set, then it doesn't. */ # define RE_DOT_NEWLINE (RE_CONTEXT_INVALID_OPS << 1) /* If this bit is set, then . doesn't match NUL. If not set, then it does. */ # define RE_DOT_NOT_NULL (RE_DOT_NEWLINE << 1) /* If this bit is set, nonmatching lists [^...] do not match newline. If not set, they do. */ # define RE_HAT_LISTS_NOT_NEWLINE (RE_DOT_NOT_NULL << 1) /* If this bit is set, either \{...\} or {...} defines an interval, depending on RE_NO_BK_BRACES. If not set, \{, \}, {, and } are literals. */ # define RE_INTERVALS (RE_HAT_LISTS_NOT_NEWLINE << 1) /* If this bit is set, +, ? and | aren't recognized as operators. If not set, they are. */ # define RE_LIMITED_OPS (RE_INTERVALS << 1) /* If this bit is set, newline is an alternation operator. If not set, newline is literal. */ # define RE_NEWLINE_ALT (RE_LIMITED_OPS << 1) /* If this bit is set, then '{...}' defines an interval, and \{ and \} are literals. If not set, then '\{...\}' defines an interval. */ # define RE_NO_BK_BRACES (RE_NEWLINE_ALT << 1) /* If this bit is set, (...) defines a group, and \( and \) are literals. If not set, \(...\) defines a group, and ( and ) are literals. */ # define RE_NO_BK_PARENS (RE_NO_BK_BRACES << 1) /* If this bit is set, then \ matches . If not set, then \ is a back-reference. */ # define RE_NO_BK_REFS (RE_NO_BK_PARENS << 1) /* If this bit is set, then | is an alternation operator, and \| is literal. If not set, then \| is an alternation operator, and | is literal. */ # define RE_NO_BK_VBAR (RE_NO_BK_REFS << 1) /* If this bit is set, then an ending range point collating higher than the starting range point, as in [z-a], is invalid. If not set, then when ending range point collates higher than the starting range point, the range is ignored. */ # define RE_NO_EMPTY_RANGES (RE_NO_BK_VBAR << 1) /* If this bit is set, then an unmatched ) is ordinary. If not set, then an unmatched ) is invalid. */ # define RE_UNMATCHED_RIGHT_PAREN_ORD (RE_NO_EMPTY_RANGES << 1) /* If this bit is set, succeed as soon as we match the whole pattern, without further backtracking. */ # define RE_NO_POSIX_BACKTRACKING (RE_UNMATCHED_RIGHT_PAREN_ORD << 1) /* If this bit is set, do not process the GNU regex operators. If not set, then the GNU regex operators are recognized. */ # define RE_NO_GNU_OPS (RE_NO_POSIX_BACKTRACKING << 1) /* If this bit is set, turn on internal regex debugging. If not set, and debugging was on, turn it off. This only works if regex.c is compiled -DDEBUG. We define this bit always, so that all that's needed to turn on debugging is to recompile regex.c; the calling code can always have this bit set, and it won't affect anything in the normal case. */ # define RE_DEBUG (RE_NO_GNU_OPS << 1) /* If this bit is set, a syntactically invalid interval is treated as a string of ordinary characters. For example, the ERE 'a{1' is treated as 'a\{1'. */ # define RE_INVALID_INTERVAL_ORD (RE_DEBUG << 1) /* If this bit is set, then ignore case when matching. If not set, then case is significant. */ # define RE_ICASE (RE_INVALID_INTERVAL_ORD << 1) /* This bit is used internally like RE_CONTEXT_INDEP_ANCHORS but only for ^, because it is difficult to scan the regex backwards to find whether ^ should be special. */ # define RE_CARET_ANCHORS_HERE (RE_ICASE << 1) /* If this bit is set, then \{ cannot be first in a regex or immediately after an alternation, open-group or \} operator. */ # define RE_CONTEXT_INVALID_DUP (RE_CARET_ANCHORS_HERE << 1) /* If this bit is set, then no_sub will be set to 1 during re_compile_pattern. */ # define RE_NO_SUB (RE_CONTEXT_INVALID_DUP << 1) #endif /* This global variable defines the particular regexp syntax to use (for some interfaces). When a regexp is compiled, the syntax used is stored in the pattern buffer, so changing this does not affect already-compiled regexps. */ extern reg_syntax_t re_syntax_options; #ifdef __USE_GNU /* Define combinations of the above bits for the standard possibilities. (The [[[ comments delimit what gets put into the Texinfo file, so don't delete them!) */ /* [[[begin syntaxes]]] */ # define RE_SYNTAX_EMACS 0 # define RE_SYNTAX_AWK \ (RE_BACKSLASH_ESCAPE_IN_LISTS | RE_DOT_NOT_NULL \ | RE_NO_BK_PARENS | RE_NO_BK_REFS \ | RE_NO_BK_VBAR | RE_NO_EMPTY_RANGES \ | RE_DOT_NEWLINE | RE_CONTEXT_INDEP_ANCHORS \ | RE_CHAR_CLASSES \ | RE_UNMATCHED_RIGHT_PAREN_ORD | RE_NO_GNU_OPS) # define RE_SYNTAX_GNU_AWK \ ((RE_SYNTAX_POSIX_EXTENDED | RE_BACKSLASH_ESCAPE_IN_LISTS \ | RE_INVALID_INTERVAL_ORD) \ & ~(RE_DOT_NOT_NULL | RE_CONTEXT_INDEP_OPS \ | RE_CONTEXT_INVALID_OPS )) # define RE_SYNTAX_POSIX_AWK \ (RE_SYNTAX_POSIX_EXTENDED | RE_BACKSLASH_ESCAPE_IN_LISTS \ | RE_INTERVALS | RE_NO_GNU_OPS \ | RE_INVALID_INTERVAL_ORD) # define RE_SYNTAX_GREP \ ((RE_SYNTAX_POSIX_BASIC | RE_NEWLINE_ALT) \ & ~(RE_CONTEXT_INVALID_DUP | RE_DOT_NOT_NULL)) # define RE_SYNTAX_EGREP \ ((RE_SYNTAX_POSIX_EXTENDED | RE_INVALID_INTERVAL_ORD | RE_NEWLINE_ALT) \ & ~(RE_CONTEXT_INVALID_OPS | RE_DOT_NOT_NULL)) /* POSIX grep -E behavior is no longer incompatible with GNU. */ # define RE_SYNTAX_POSIX_EGREP \ RE_SYNTAX_EGREP /* P1003.2/D11.2, section 4.20.7.1, lines 5078ff. */ # define RE_SYNTAX_ED RE_SYNTAX_POSIX_BASIC # define RE_SYNTAX_SED RE_SYNTAX_POSIX_BASIC /* Syntax bits common to both basic and extended POSIX regex syntax. */ # define _RE_SYNTAX_POSIX_COMMON \ (RE_CHAR_CLASSES | RE_DOT_NEWLINE | RE_DOT_NOT_NULL \ | RE_INTERVALS | RE_NO_EMPTY_RANGES) # define RE_SYNTAX_POSIX_BASIC \ (_RE_SYNTAX_POSIX_COMMON | RE_BK_PLUS_QM | RE_CONTEXT_INVALID_DUP) /* Differs from ..._POSIX_BASIC only in that RE_BK_PLUS_QM becomes RE_LIMITED_OPS, i.e., \? \+ \| are not recognized. Actually, this isn't minimal, since other operators, such as \`, aren't disabled. */ # define RE_SYNTAX_POSIX_MINIMAL_BASIC \ (_RE_SYNTAX_POSIX_COMMON | RE_LIMITED_OPS) # define RE_SYNTAX_POSIX_EXTENDED \ (_RE_SYNTAX_POSIX_COMMON | RE_CONTEXT_INDEP_ANCHORS \ | RE_CONTEXT_INDEP_OPS | RE_NO_BK_BRACES \ | RE_NO_BK_PARENS | RE_NO_BK_VBAR \ | RE_CONTEXT_INVALID_OPS | RE_UNMATCHED_RIGHT_PAREN_ORD) /* Differs from ..._POSIX_EXTENDED in that RE_CONTEXT_INDEP_OPS is removed and RE_NO_BK_REFS is added. */ # define RE_SYNTAX_POSIX_MINIMAL_EXTENDED \ (_RE_SYNTAX_POSIX_COMMON | RE_CONTEXT_INDEP_ANCHORS \ | RE_CONTEXT_INVALID_OPS | RE_NO_BK_BRACES \ | RE_NO_BK_PARENS | RE_NO_BK_REFS \ | RE_NO_BK_VBAR | RE_UNMATCHED_RIGHT_PAREN_ORD) /* [[[end syntaxes]]] */ /* Maximum number of duplicates an interval can allow. POSIX-conforming systems might define this in , but we want our value, so remove any previous define. */ # ifdef _REGEX_INCLUDE_LIMITS_H # include # endif # ifdef RE_DUP_MAX # undef RE_DUP_MAX # endif /* RE_DUP_MAX is 2**15 - 1 because an earlier implementation stored the counter as a 2-byte signed integer. This is no longer true, so RE_DUP_MAX could be increased to (INT_MAX / 10 - 1), or to ((SIZE_MAX - 9) / 10) if _REGEX_LARGE_OFFSETS is defined. However, there would be a huge performance problem if someone actually used a pattern like a\{214748363\}, so RE_DUP_MAX retains its historical value. */ # define RE_DUP_MAX (0x7fff) #endif /* POSIX 'cflags' bits (i.e., information for 'regcomp'). */ /* If this bit is set, then use extended regular expression syntax. If not set, then use basic regular expression syntax. */ #define REG_EXTENDED 1 /* If this bit is set, then ignore case when matching. If not set, then case is significant. */ #define REG_ICASE (1 << 1) /* If this bit is set, then anchors do not match at newline characters in the string. If not set, then anchors do match at newlines. */ #define REG_NEWLINE (1 << 2) /* If this bit is set, then report only success or fail in regexec. If not set, then returns differ between not matching and errors. */ #define REG_NOSUB (1 << 3) /* POSIX 'eflags' bits (i.e., information for regexec). */ /* If this bit is set, then the beginning-of-line operator doesn't match the beginning of the string (presumably because it's not the beginning of a line). If not set, then the beginning-of-line operator does match the beginning of the string. */ #define REG_NOTBOL 1 /* Like REG_NOTBOL, except for the end-of-line. */ #define REG_NOTEOL (1 << 1) /* Use PMATCH[0] to delimit the start and end of the search in the buffer. */ #define REG_STARTEND (1 << 2) /* If any error codes are removed, changed, or added, update the '__re_error_msgid' table in regcomp.c. */ typedef enum { _REG_ENOSYS = -1, /* This will never happen for this implementation. */ _REG_NOERROR = 0, /* Success. */ _REG_NOMATCH, /* Didn't find a match (for regexec). */ /* POSIX regcomp return error codes. (In the order listed in the standard.) */ _REG_BADPAT, /* Invalid pattern. */ _REG_ECOLLATE, /* Invalid collating element. */ _REG_ECTYPE, /* Invalid character class name. */ _REG_EESCAPE, /* Trailing backslash. */ _REG_ESUBREG, /* Invalid back reference. */ _REG_EBRACK, /* Unmatched left bracket. */ _REG_EPAREN, /* Parenthesis imbalance. */ _REG_EBRACE, /* Unmatched \{. */ _REG_BADBR, /* Invalid contents of \{\}. */ _REG_ERANGE, /* Invalid range end. */ _REG_ESPACE, /* Ran out of memory. */ _REG_BADRPT, /* No preceding re for repetition op. */ /* Error codes we've added. */ _REG_EEND, /* Premature end. */ _REG_ESIZE, /* Too large (e.g., repeat count too large). */ _REG_ERPAREN /* Unmatched ) or \); not returned from regcomp. */ } reg_errcode_t; #if defined _XOPEN_SOURCE || defined __USE_XOPEN2K # define REG_ENOSYS _REG_ENOSYS #endif #define REG_NOERROR _REG_NOERROR #define REG_NOMATCH _REG_NOMATCH #define REG_BADPAT _REG_BADPAT #define REG_ECOLLATE _REG_ECOLLATE #define REG_ECTYPE _REG_ECTYPE #define REG_EESCAPE _REG_EESCAPE #define REG_ESUBREG _REG_ESUBREG #define REG_EBRACK _REG_EBRACK #define REG_EPAREN _REG_EPAREN #define REG_EBRACE _REG_EBRACE #define REG_BADBR _REG_BADBR #define REG_ERANGE _REG_ERANGE #define REG_ESPACE _REG_ESPACE #define REG_BADRPT _REG_BADRPT #define REG_EEND _REG_EEND #define REG_ESIZE _REG_ESIZE #define REG_ERPAREN _REG_ERPAREN /* This data structure represents a compiled pattern. Before calling the pattern compiler, the fields 'buffer', 'allocated', 'fastmap', and 'translate' can be set. After the pattern has been compiled, the fields 're_nsub', 'not_bol' and 'not_eol' are available. All other fields are private to the regex routines. */ #ifndef RE_TRANSLATE_TYPE # define __RE_TRANSLATE_TYPE unsigned char * # ifdef __USE_GNU # define RE_TRANSLATE_TYPE __RE_TRANSLATE_TYPE # endif #endif #ifdef __USE_GNU # define __REPB_PREFIX(name) name #else # define __REPB_PREFIX(name) __##name #endif struct re_pattern_buffer { /* Space that holds the compiled pattern. The type 'struct re_dfa_t' is private and is not declared here. */ struct re_dfa_t *__REPB_PREFIX(buffer); /* Number of bytes to which 'buffer' points. */ __re_long_size_t __REPB_PREFIX(allocated); /* Number of bytes actually used in 'buffer'. */ __re_long_size_t __REPB_PREFIX(used); /* Syntax setting with which the pattern was compiled. */ reg_syntax_t __REPB_PREFIX(syntax); /* Pointer to a fastmap, if any, otherwise zero. re_search uses the fastmap, if there is one, to skip over impossible starting points for matches. */ char *__REPB_PREFIX(fastmap); /* Either a translate table to apply to all characters before comparing them, or zero for no translation. The translation is applied to a pattern when it is compiled and to a string when it is matched. */ __RE_TRANSLATE_TYPE __REPB_PREFIX(translate); /* Number of subexpressions found by the compiler. */ size_t re_nsub; /* Zero if this pattern cannot match the empty string, one else. Well, in truth it's used only in 're_search_2', to see whether or not we should use the fastmap, so we don't set this absolutely perfectly; see 're_compile_fastmap' (the "duplicate" case). */ unsigned __REPB_PREFIX(can_be_null) : 1; /* If REGS_UNALLOCATED, allocate space in the 'regs' structure for 'max (RE_NREGS, re_nsub + 1)' groups. If REGS_REALLOCATE, reallocate space if necessary. If REGS_FIXED, use what's there. */ #ifdef __USE_GNU # define REGS_UNALLOCATED 0 # define REGS_REALLOCATE 1 # define REGS_FIXED 2 #endif unsigned __REPB_PREFIX(regs_allocated) : 2; /* Set to zero when 're_compile_pattern' compiles a pattern; set to one by 're_compile_fastmap' if it updates the fastmap. */ unsigned __REPB_PREFIX(fastmap_accurate) : 1; /* If set, 're_match_2' does not return information about subexpressions. */ unsigned __REPB_PREFIX(no_sub) : 1; /* If set, a beginning-of-line anchor doesn't match at the beginning of the string. */ unsigned __REPB_PREFIX(not_bol) : 1; /* Similarly for an end-of-line anchor. */ unsigned __REPB_PREFIX(not_eol) : 1; /* If true, an anchor at a newline matches. */ unsigned __REPB_PREFIX(newline_anchor) : 1; }; typedef struct re_pattern_buffer regex_t; /* Type for byte offsets within the string. POSIX mandates this. */ #ifdef _REGEX_LARGE_OFFSETS /* POSIX 1003.1-2008 requires that regoff_t be at least as wide as ptrdiff_t and ssize_t. We don't know of any hosts where ptrdiff_t is wider than ssize_t, so ssize_t is safe. ptrdiff_t is not visible here, so use ssize_t. */ typedef ssize_t regoff_t; #else /* The traditional GNU regex implementation mishandles strings longer than INT_MAX. */ typedef int regoff_t; #endif #ifdef __USE_GNU /* This is the structure we store register match data in. See regex.texinfo for a full description of what registers match. */ struct re_registers { __re_size_t num_regs; regoff_t *start; regoff_t *end; }; /* If 'regs_allocated' is REGS_UNALLOCATED in the pattern buffer, 're_match_2' returns information about at least this many registers the first time a 'regs' structure is passed. */ # ifndef RE_NREGS # define RE_NREGS 30 # endif #endif /* POSIX specification for registers. Aside from the different names than 're_registers', POSIX uses an array of structures, instead of a structure of arrays. */ typedef struct { regoff_t rm_so; /* Byte offset from string's start to substring's start. */ regoff_t rm_eo; /* Byte offset from string's start to substring's end. */ } regmatch_t; /* Declarations for routines. */ #ifdef __USE_GNU /* Sets the current default syntax to SYNTAX, and return the old syntax. You can also simply assign to the 're_syntax_options' variable. */ extern reg_syntax_t re_set_syntax (reg_syntax_t __syntax); /* Compile the regular expression PATTERN, with length LENGTH and syntax given by the global 're_syntax_options', into the buffer BUFFER. Return NULL if successful, and an error string if not. To free the allocated storage, you must call 'regfree' on BUFFER. Note that the translate table must either have been initialized by 'regcomp', with a malloc'ed value, or set to NULL before calling 'regfree'. */ extern const char *re_compile_pattern (const char *__pattern, size_t __length, struct re_pattern_buffer *__buffer); /* Compile a fastmap for the compiled pattern in BUFFER; used to accelerate searches. Return 0 if successful and -2 if was an internal error. */ extern int re_compile_fastmap (struct re_pattern_buffer *__buffer); /* Search in the string STRING (with length LENGTH) for the pattern compiled into BUFFER. Start searching at position START, for RANGE characters. Return the starting position of the match, -1 for no match, or -2 for an internal error. Also return register information in REGS (if REGS and BUFFER->no_sub are nonzero). */ extern regoff_t re_search (struct re_pattern_buffer *__buffer, const char *__String, regoff_t __length, regoff_t __start, regoff_t __range, struct re_registers *__regs); /* Like 're_search', but search in the concatenation of STRING1 and STRING2. Also, stop searching at index START + STOP. */ extern regoff_t re_search_2 (struct re_pattern_buffer *__buffer, const char *__string1, regoff_t __length1, const char *__string2, regoff_t __length2, regoff_t __start, regoff_t __range, struct re_registers *__regs, regoff_t __stop); /* Like 're_search', but return how many characters in STRING the regexp in BUFFER matched, starting at position START. */ extern regoff_t re_match (struct re_pattern_buffer *__buffer, const char *__String, regoff_t __length, regoff_t __start, struct re_registers *__regs); /* Relates to 're_match' as 're_search_2' relates to 're_search'. */ extern regoff_t re_match_2 (struct re_pattern_buffer *__buffer, const char *__string1, regoff_t __length1, const char *__string2, regoff_t __length2, regoff_t __start, struct re_registers *__regs, regoff_t __stop); /* Set REGS to hold NUM_REGS registers, storing them in STARTS and ENDS. Subsequent matches using BUFFER and REGS will use this memory for recording register information. STARTS and ENDS must be allocated with malloc, and must each be at least 'NUM_REGS * sizeof (regoff_t)' bytes long. If NUM_REGS == 0, then subsequent matches should allocate their own register data. Unless this function is called, the first search or match using BUFFER will allocate its own register data, without freeing the old data. */ extern void re_set_registers (struct re_pattern_buffer *__buffer, struct re_registers *__regs, __re_size_t __num_regs, regoff_t *__starts, regoff_t *__ends); #endif /* Use GNU */ #if defined _REGEX_RE_COMP || (defined _LIBC && defined __USE_MISC) # ifndef _CRAY /* 4.2 bsd compatibility. */ extern char *re_comp (const char *); extern int re_exec (const char *); # endif #endif /* GCC 2.95 and later have "__restrict"; C99 compilers have "restrict", and "configure" may have defined "restrict". Other compilers use __restrict, __restrict__, and _Restrict, and 'configure' might #define 'restrict' to those words, so pick a different name. */ #ifndef _Restrict_ # if 199901L <= __STDC_VERSION__ # define _Restrict_ restrict # elif 2 < __GNUC__ || (2 == __GNUC__ && 95 <= __GNUC_MINOR__) # define _Restrict_ __restrict # else # define _Restrict_ # endif #endif /* gcc 3.1 and up support the [restrict] syntax. Don't trust sys/cdefs.h's definition of __restrict_arr, though, as it mishandles gcc -ansi -pedantic. */ #ifndef _Restrict_arr_ # if ((199901L <= __STDC_VERSION__ \ || ((3 < __GNUC__ || (3 == __GNUC__ && 1 <= __GNUC_MINOR__)) \ && !defined __STRICT_ANSI__)) \ && !defined __GNUG__) # define _Restrict_arr_ _Restrict_ # else # define _Restrict_arr_ # endif #endif /* POSIX compatibility. */ extern int regcomp (regex_t *_Restrict_ __preg, const char *_Restrict_ __pattern, int __cflags); extern int regexec (const regex_t *_Restrict_ __preg, const char *_Restrict_ __String, size_t __nmatch, regmatch_t __pmatch[_Restrict_arr_], int __eflags); extern size_t regerror (int __errcode, const regex_t *_Restrict_ __preg, char *_Restrict_ __errbuf, size_t __errbuf_size); extern void regfree (regex_t *__preg); #ifdef __cplusplus } #endif /* C++ */ #endif /* regex.h */ gnuastro-0.2.33-8a3b/bootstrapped/lib/rawmemchr.valgrind0000644000175000017500000000040313004436754020111 00000000000000# Suppress a valgrind message about use of uninitialized memory in rawmemchr(). # This use is OK because it provides only a speedup. { rawmemchr-value4 Memcheck:Value4 fun:rawmemchr } { rawmemchr-value8 Memcheck:Value8 fun:rawmemchr } gnuastro-0.2.33-8a3b/bootstrapped/lib/nproc.h0000644000175000017500000000331013004436754015666 00000000000000/* Detect the number of processors. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Glen Lenker and Bruno Haible. */ /* Allow the use in C++ code. */ #ifdef __cplusplus extern "C" { #endif /* A "processor" in this context means a thread execution unit, that is either - an execution core in a (possibly multi-core) chip, in a (possibly multi- chip) module, in a single computer, or - a thread execution unit inside a core (hyper-threading, see ). Which of the two definitions is used, is unspecified. */ enum nproc_query { NPROC_ALL, /* total number of processors */ NPROC_CURRENT, /* processors available to the current process */ NPROC_CURRENT_OVERRIDABLE /* likewise, but overridable through the OMP_NUM_THREADS environment variable */ }; /* Return the total number of processors. The result is guaranteed to be at least 1. */ extern unsigned long int num_processors (enum nproc_query query); #ifdef __cplusplus } #endif /* C++ */ gnuastro-0.2.33-8a3b/bootstrapped/lib/msvc-nothrow.h0000644000175000017500000000301013004436754017210 00000000000000/* Wrappers that don't throw invalid parameter notifications with MSVC runtime libraries. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _MSVC_NOTHROW_H #define _MSVC_NOTHROW_H /* With MSVC runtime libraries with the "invalid parameter handler" concept, functions like fprintf(), dup2(), or close() crash when the caller passes an invalid argument. But POSIX wants error codes (such as EINVAL or EBADF) instead. This file defines wrappers that turn such an invalid parameter notification into an error code. */ #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Get original declaration of _get_osfhandle. */ # include # if HAVE_MSVC_INVALID_PARAMETER_HANDLER /* Override _get_osfhandle. */ extern intptr_t _gl_nothrow_get_osfhandle (int fd); # define _get_osfhandle _gl_nothrow_get_osfhandle # endif #endif #endif /* _MSVC_NOTHROW_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/msvc-inval.h0000644000175000017500000002113513004436754016631 00000000000000/* Invalid parameter handler for MSVC runtime libraries. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _MSVC_INVAL_H #define _MSVC_INVAL_H /* With MSVC runtime libraries with the "invalid parameter handler" concept, functions like fprintf(), dup2(), or close() crash when the caller passes an invalid argument. But POSIX wants error codes (such as EINVAL or EBADF) instead. This file defines macros that turn such an invalid parameter notification into a non-local exit. An error code can then be produced at the target of this exit. You can thus write code like TRY_MSVC_INVAL { } CATCH_MSVC_INVAL { } DONE_MSVC_INVAL; This entire block expands to a single statement. The handling of invalid parameters can be done in three ways: * The default way, which is reasonable for programs (not libraries): AC_DEFINE([MSVC_INVALID_PARAMETER_HANDLING], [DEFAULT_HANDLING]) * The way for libraries that make "hairy" calls (like close(-1), or fclose(fp) where fileno(fp) is closed, or simply getdtablesize()): AC_DEFINE([MSVC_INVALID_PARAMETER_HANDLING], [HAIRY_LIBRARY_HANDLING]) * The way for libraries that make no "hairy" calls: AC_DEFINE([MSVC_INVALID_PARAMETER_HANDLING], [SANE_LIBRARY_HANDLING]) */ #define DEFAULT_HANDLING 0 #define HAIRY_LIBRARY_HANDLING 1 #define SANE_LIBRARY_HANDLING 2 #if HAVE_MSVC_INVALID_PARAMETER_HANDLER \ && !(MSVC_INVALID_PARAMETER_HANDLING == SANE_LIBRARY_HANDLING) /* A native Windows platform with the "invalid parameter handler" concept, and either DEFAULT_HANDLING or HAIRY_LIBRARY_HANDLING. */ # if MSVC_INVALID_PARAMETER_HANDLING == DEFAULT_HANDLING /* Default handling. */ # ifdef __cplusplus extern "C" { # endif /* Ensure that the invalid parameter handler in installed that just returns. Because we assume no other part of the program installs a different invalid parameter handler, this solution is multithread-safe. */ extern void gl_msvc_inval_ensure_handler (void); # ifdef __cplusplus } # endif # define TRY_MSVC_INVAL \ do \ { \ gl_msvc_inval_ensure_handler (); \ if (1) # define CATCH_MSVC_INVAL \ else # define DONE_MSVC_INVAL \ } \ while (0) # else /* Handling for hairy libraries. */ # include /* Gnulib can define its own status codes, as described in the page "Raising Software Exceptions" on microsoft.com . Our status codes are composed of - 0xE0000000, mandatory for all user-defined status codes, - 0x474E550, a API identifier ("GNU"), - 0, 1, 2, ..., used to distinguish different status codes from the same API. */ # define STATUS_GNULIB_INVALID_PARAMETER (0xE0000000 + 0x474E550 + 0) # if defined _MSC_VER /* A compiler that supports __try/__except, as described in the page "try-except statement" on microsoft.com . With __try/__except, we can use the multithread-safe exception handling. */ # ifdef __cplusplus extern "C" { # endif /* Ensure that the invalid parameter handler in installed that raises a software exception with code STATUS_GNULIB_INVALID_PARAMETER. Because we assume no other part of the program installs a different invalid parameter handler, this solution is multithread-safe. */ extern void gl_msvc_inval_ensure_handler (void); # ifdef __cplusplus } # endif # define TRY_MSVC_INVAL \ do \ { \ gl_msvc_inval_ensure_handler (); \ __try # define CATCH_MSVC_INVAL \ __except (GetExceptionCode () == STATUS_GNULIB_INVALID_PARAMETER \ ? EXCEPTION_EXECUTE_HANDLER \ : EXCEPTION_CONTINUE_SEARCH) # define DONE_MSVC_INVAL \ } \ while (0) # else /* Any compiler. We can only use setjmp/longjmp. */ # include # ifdef __cplusplus extern "C" { # endif struct gl_msvc_inval_per_thread { /* The restart that will resume execution at the code between CATCH_MSVC_INVAL and DONE_MSVC_INVAL. It is enabled only between TRY_MSVC_INVAL and CATCH_MSVC_INVAL. */ jmp_buf restart; /* Tells whether the contents of restart is valid. */ int restart_valid; }; /* Ensure that the invalid parameter handler in installed that passes control to the gl_msvc_inval_restart if it is valid, or raises a software exception with code STATUS_GNULIB_INVALID_PARAMETER otherwise. Because we assume no other part of the program installs a different invalid parameter handler, this solution is multithread-safe. */ extern void gl_msvc_inval_ensure_handler (void); /* Return a pointer to the per-thread data for the current thread. */ extern struct gl_msvc_inval_per_thread *gl_msvc_inval_current (void); # ifdef __cplusplus } # endif # define TRY_MSVC_INVAL \ do \ { \ struct gl_msvc_inval_per_thread *msvc_inval_current; \ gl_msvc_inval_ensure_handler (); \ msvc_inval_current = gl_msvc_inval_current (); \ /* First, initialize gl_msvc_inval_restart. */ \ if (setjmp (msvc_inval_current->restart) == 0) \ { \ /* Then, mark it as valid. */ \ msvc_inval_current->restart_valid = 1; # define CATCH_MSVC_INVAL \ /* Execution completed. \ Mark gl_msvc_inval_restart as invalid. */ \ msvc_inval_current->restart_valid = 0; \ } \ else \ { \ /* Execution triggered an invalid parameter notification. \ Mark gl_msvc_inval_restart as invalid. */ \ msvc_inval_current->restart_valid = 0; # define DONE_MSVC_INVAL \ } \ } \ while (0) # endif # endif #else /* A platform that does not need to the invalid parameter handler, or when SANE_LIBRARY_HANDLING is desired. */ /* The braces here avoid GCC warnings like "warning: suggest explicit braces to avoid ambiguous 'else'". */ # define TRY_MSVC_INVAL \ do \ { \ if (1) # define CATCH_MSVC_INVAL \ else # define DONE_MSVC_INVAL \ } \ while (0) #endif #endif /* _MSVC_INVAL_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/memchr.valgrind0000644000175000017500000000065213004436754017405 00000000000000# Suppress a valgrind message about use of uninitialized memory in memchr(). # POSIX states that when the character is found, memchr must not read extra # bytes in an overestimated length (for example, where memchr is used to # implement strnlen). However, we use a safe word read to provide a speedup. { memchr-value4 Memcheck:Value4 fun:rpl_memchr } { memchr-value8 Memcheck:Value8 fun:rpl_memchr } gnuastro-0.2.33-8a3b/bootstrapped/lib/mbtowc-impl.h0000644000175000017500000000262613004436754017010 00000000000000/* Convert multibyte character to wide character. Copyright (C) 2011-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2011. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* We don't need a static internal state, because the encoding is not state dependent, and when mbrtowc returns (size_t)(-2). we throw the result away. */ int mbtowc (wchar_t *pwc, const char *s, size_t n) { if (s == NULL) return 0; else { mbstate_t state; wchar_t wc; size_t result; memset (&state, 0, sizeof (mbstate_t)); result = mbrtowc (&wc, s, n, &state); if (result == (size_t)-1 || result == (size_t)-2) { errno = EILSEQ; return -1; } if (pwc != NULL) *pwc = wc; return (wc == 0 ? 0 : result); } } gnuastro-0.2.33-8a3b/bootstrapped/lib/math.in.h0000644000175000017500000020020213004436754016102 00000000000000/* A GNU-like . Copyright (C) 2002-2003, 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _@GUARD_PREFIX@_MATH_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ #ifndef _@GUARD_PREFIX@_MATH_H #define _@GUARD_PREFIX@_MATH_H #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef _GL_MATH_INLINE # define _GL_MATH_INLINE _GL_INLINE #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ #ifdef __cplusplus /* Helper macros to define type-generic function FUNC as overloaded functions, rather than as macros like in C. POSIX declares these with an argument of real-floating (that is, one of float, double, or long double). */ # define _GL_MATH_CXX_REAL_FLOATING_DECL_1(func) \ static inline int \ _gl_cxx_ ## func ## f (float f) \ { \ return func (f); \ } \ static inline int \ _gl_cxx_ ## func ## d (double d) \ { \ return func (d); \ } \ static inline int \ _gl_cxx_ ## func ## l (long double l) \ { \ return func (l); \ } # define _GL_MATH_CXX_REAL_FLOATING_DECL_2(func) \ inline int \ func (float f) \ { \ return _gl_cxx_ ## func ## f (f); \ } \ inline int \ func (double d) \ { \ return _gl_cxx_ ## func ## d (d); \ } \ inline int \ func (long double l) \ { \ return _gl_cxx_ ## func ## l (l); \ } #endif /* Helper macros to define a portability warning for the classification macro FUNC called with VALUE. POSIX declares the classification macros with an argument of real-floating (that is, one of float, double, or long double). */ #define _GL_WARN_REAL_FLOATING_DECL(func) \ _GL_MATH_INLINE int \ rpl_ ## func ## f (float f) \ { \ return func (f); \ } \ _GL_MATH_INLINE int \ rpl_ ## func ## d (double d) \ { \ return func (d); \ } \ _GL_MATH_INLINE int \ rpl_ ## func ## l (long double l) \ { \ return func (l); \ } \ _GL_WARN_ON_USE (rpl_ ## func ## f, #func " is unportable - " \ "use gnulib module " #func " for portability"); \ _GL_WARN_ON_USE (rpl_ ## func ## d, #func " is unportable - " \ "use gnulib module " #func " for portability"); \ _GL_WARN_ON_USE (rpl_ ## func ## l, #func " is unportable - " \ "use gnulib module " #func " for portability") #define _GL_WARN_REAL_FLOATING_IMPL(func, value) \ (sizeof (value) == sizeof (float) ? rpl_ ## func ## f (value) \ : sizeof (value) == sizeof (double) ? rpl_ ## func ## d (value) \ : rpl_ ## func ## l (value)) #if @REPLACE_ITOLD@ /* Pull in a function that fixes the 'int' to 'long double' conversion of glibc 2.7. */ _GL_EXTERN_C void _Qp_itoq (long double *, int); static void (*_gl_math_fix_itold) (long double *, int) = _Qp_itoq; #endif /* POSIX allows platforms that don't support NAN. But all major machines in the past 15 years have supported something close to IEEE NaN, so we define this unconditionally. We also must define it on platforms like Solaris 10, where NAN is present but defined as a function pointer rather than a floating point constant. */ #if !defined NAN || @REPLACE_NAN@ # if !GNULIB_defined_NAN # undef NAN /* The Compaq (ex-DEC) C 6.4 compiler and the Microsoft MSVC 9 compiler choke on the expression 0.0 / 0.0. */ # if defined __DECC || defined _MSC_VER _GL_MATH_INLINE float _NaN () { static float zero = 0.0f; return zero / zero; } # define NAN (_NaN()) # else # define NAN (0.0f / 0.0f) # endif # define GNULIB_defined_NAN 1 # endif #endif /* Solaris 10 defines HUGE_VAL, but as a function pointer rather than a floating point constant. */ #if @REPLACE_HUGE_VAL@ # undef HUGE_VALF # define HUGE_VALF (1.0f / 0.0f) # undef HUGE_VAL # define HUGE_VAL (1.0 / 0.0) # undef HUGE_VALL # define HUGE_VALL (1.0L / 0.0L) #endif /* HUGE_VALF is a 'float' Infinity. */ #ifndef HUGE_VALF # if defined _MSC_VER /* The Microsoft MSVC 9 compiler chokes on the expression 1.0f / 0.0f. */ # define HUGE_VALF (1e25f * 1e25f) # else # define HUGE_VALF (1.0f / 0.0f) # endif #endif /* HUGE_VAL is a 'double' Infinity. */ #ifndef HUGE_VAL # if defined _MSC_VER /* The Microsoft MSVC 9 compiler chokes on the expression 1.0 / 0.0. */ # define HUGE_VAL (1e250 * 1e250) # else # define HUGE_VAL (1.0 / 0.0) # endif #endif /* HUGE_VALL is a 'long double' Infinity. */ #ifndef HUGE_VALL # if defined _MSC_VER /* The Microsoft MSVC 9 compiler chokes on the expression 1.0L / 0.0L. */ # define HUGE_VALL (1e250L * 1e250L) # else # define HUGE_VALL (1.0L / 0.0L) # endif #endif /* Ensure FP_ILOGB0 and FP_ILOGBNAN are defined. */ #if !(defined FP_ILOGB0 && defined FP_ILOGBNAN) # if defined __NetBSD__ || defined __sgi /* NetBSD, IRIX 6.5: match what ilogb() does */ # define FP_ILOGB0 (- 2147483647 - 1) /* INT_MIN */ # define FP_ILOGBNAN (- 2147483647 - 1) /* INT_MIN */ # elif defined _AIX /* AIX 5.1: match what ilogb() does in AIX >= 5.2 */ # define FP_ILOGB0 (- 2147483647 - 1) /* INT_MIN */ # define FP_ILOGBNAN 2147483647 /* INT_MAX */ # elif defined __sun /* Solaris 9: match what ilogb() does */ # define FP_ILOGB0 (- 2147483647) /* - INT_MAX */ # define FP_ILOGBNAN 2147483647 /* INT_MAX */ # else /* Gnulib defined values. */ # define FP_ILOGB0 (- 2147483647) /* - INT_MAX */ # define FP_ILOGBNAN (- 2147483647 - 1) /* INT_MIN */ # endif #endif #if @GNULIB_ACOSF@ # if !@HAVE_ACOSF@ # undef acosf _GL_FUNCDECL_SYS (acosf, float, (float x)); # endif _GL_CXXALIAS_SYS (acosf, float, (float x)); _GL_CXXALIASWARN (acosf); #elif defined GNULIB_POSIXCHECK # undef acosf # if HAVE_RAW_DECL_ACOSF _GL_WARN_ON_USE (acosf, "acosf is unportable - " "use gnulib module acosf for portability"); # endif #endif #if @GNULIB_ACOSL@ # if !@HAVE_ACOSL@ || !@HAVE_DECL_ACOSL@ # undef acosl _GL_FUNCDECL_SYS (acosl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (acosl, long double, (long double x)); _GL_CXXALIASWARN (acosl); #elif defined GNULIB_POSIXCHECK # undef acosl # if HAVE_RAW_DECL_ACOSL _GL_WARN_ON_USE (acosl, "acosl is unportable - " "use gnulib module acosl for portability"); # endif #endif #if @GNULIB_ASINF@ # if !@HAVE_ASINF@ # undef asinf _GL_FUNCDECL_SYS (asinf, float, (float x)); # endif _GL_CXXALIAS_SYS (asinf, float, (float x)); _GL_CXXALIASWARN (asinf); #elif defined GNULIB_POSIXCHECK # undef asinf # if HAVE_RAW_DECL_ASINF _GL_WARN_ON_USE (asinf, "asinf is unportable - " "use gnulib module asinf for portability"); # endif #endif #if @GNULIB_ASINL@ # if !@HAVE_ASINL@ || !@HAVE_DECL_ASINL@ # undef asinl _GL_FUNCDECL_SYS (asinl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (asinl, long double, (long double x)); _GL_CXXALIASWARN (asinl); #elif defined GNULIB_POSIXCHECK # undef asinl # if HAVE_RAW_DECL_ASINL _GL_WARN_ON_USE (asinl, "asinl is unportable - " "use gnulib module asinl for portability"); # endif #endif #if @GNULIB_ATANF@ # if !@HAVE_ATANF@ # undef atanf _GL_FUNCDECL_SYS (atanf, float, (float x)); # endif _GL_CXXALIAS_SYS (atanf, float, (float x)); _GL_CXXALIASWARN (atanf); #elif defined GNULIB_POSIXCHECK # undef atanf # if HAVE_RAW_DECL_ATANF _GL_WARN_ON_USE (atanf, "atanf is unportable - " "use gnulib module atanf for portability"); # endif #endif #if @GNULIB_ATANL@ # if !@HAVE_ATANL@ || !@HAVE_DECL_ATANL@ # undef atanl _GL_FUNCDECL_SYS (atanl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (atanl, long double, (long double x)); _GL_CXXALIASWARN (atanl); #elif defined GNULIB_POSIXCHECK # undef atanl # if HAVE_RAW_DECL_ATANL _GL_WARN_ON_USE (atanl, "atanl is unportable - " "use gnulib module atanl for portability"); # endif #endif #if @GNULIB_ATAN2F@ # if !@HAVE_ATAN2F@ # undef atan2f _GL_FUNCDECL_SYS (atan2f, float, (float y, float x)); # endif _GL_CXXALIAS_SYS (atan2f, float, (float y, float x)); _GL_CXXALIASWARN (atan2f); #elif defined GNULIB_POSIXCHECK # undef atan2f # if HAVE_RAW_DECL_ATAN2F _GL_WARN_ON_USE (atan2f, "atan2f is unportable - " "use gnulib module atan2f for portability"); # endif #endif #if @GNULIB_CBRTF@ # if @REPLACE_CBRTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef cbrtf # define cbrtf rpl_cbrtf # endif _GL_FUNCDECL_RPL (cbrtf, float, (float x)); _GL_CXXALIAS_RPL (cbrtf, float, (float x)); # else # if !@HAVE_DECL_CBRTF@ _GL_FUNCDECL_SYS (cbrtf, float, (float x)); # endif _GL_CXXALIAS_SYS (cbrtf, float, (float x)); # endif _GL_CXXALIASWARN (cbrtf); #elif defined GNULIB_POSIXCHECK # undef cbrtf # if HAVE_RAW_DECL_CBRTF _GL_WARN_ON_USE (cbrtf, "cbrtf is unportable - " "use gnulib module cbrtf for portability"); # endif #endif #if @GNULIB_CBRT@ # if !@HAVE_CBRT@ _GL_FUNCDECL_SYS (cbrt, double, (double x)); # endif _GL_CXXALIAS_SYS (cbrt, double, (double x)); _GL_CXXALIASWARN (cbrt); #elif defined GNULIB_POSIXCHECK # undef cbrt # if HAVE_RAW_DECL_CBRT _GL_WARN_ON_USE (cbrt, "cbrt is unportable - " "use gnulib module cbrt for portability"); # endif #endif #if @GNULIB_CBRTL@ # if @REPLACE_CBRTL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef cbrtl # define cbrtl rpl_cbrtl # endif _GL_FUNCDECL_RPL (cbrtl, long double, (long double x)); _GL_CXXALIAS_RPL (cbrtl, long double, (long double x)); # else # if !@HAVE_DECL_CBRTL@ _GL_FUNCDECL_SYS (cbrtl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (cbrtl, long double, (long double x)); # endif _GL_CXXALIASWARN (cbrtl); #elif defined GNULIB_POSIXCHECK # undef cbrtl # if HAVE_RAW_DECL_CBRTL _GL_WARN_ON_USE (cbrtl, "cbrtl is unportable - " "use gnulib module cbrtl for portability"); # endif #endif #if @GNULIB_CEILF@ # if @REPLACE_CEILF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ceilf # define ceilf rpl_ceilf # endif _GL_FUNCDECL_RPL (ceilf, float, (float x)); _GL_CXXALIAS_RPL (ceilf, float, (float x)); # else # if !@HAVE_DECL_CEILF@ # undef ceilf _GL_FUNCDECL_SYS (ceilf, float, (float x)); # endif _GL_CXXALIAS_SYS (ceilf, float, (float x)); # endif _GL_CXXALIASWARN (ceilf); #elif defined GNULIB_POSIXCHECK # undef ceilf # if HAVE_RAW_DECL_CEILF _GL_WARN_ON_USE (ceilf, "ceilf is unportable - " "use gnulib module ceilf for portability"); # endif #endif #if @GNULIB_CEIL@ # if @REPLACE_CEIL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ceil # define ceil rpl_ceil # endif _GL_FUNCDECL_RPL (ceil, double, (double x)); _GL_CXXALIAS_RPL (ceil, double, (double x)); # else _GL_CXXALIAS_SYS (ceil, double, (double x)); # endif _GL_CXXALIASWARN (ceil); #endif #if @GNULIB_CEILL@ # if @REPLACE_CEILL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ceill # define ceill rpl_ceill # endif _GL_FUNCDECL_RPL (ceill, long double, (long double x)); _GL_CXXALIAS_RPL (ceill, long double, (long double x)); # else # if !@HAVE_DECL_CEILL@ # undef ceill _GL_FUNCDECL_SYS (ceill, long double, (long double x)); # endif _GL_CXXALIAS_SYS (ceill, long double, (long double x)); # endif _GL_CXXALIASWARN (ceill); #elif defined GNULIB_POSIXCHECK # undef ceill # if HAVE_RAW_DECL_CEILL _GL_WARN_ON_USE (ceill, "ceill is unportable - " "use gnulib module ceill for portability"); # endif #endif #if @GNULIB_COPYSIGNF@ # if !@HAVE_DECL_COPYSIGNF@ _GL_FUNCDECL_SYS (copysignf, float, (float x, float y)); # endif _GL_CXXALIAS_SYS (copysignf, float, (float x, float y)); _GL_CXXALIASWARN (copysignf); #elif defined GNULIB_POSIXCHECK # undef copysignf # if HAVE_RAW_DECL_COPYSIGNF _GL_WARN_ON_USE (copysignf, "copysignf is unportable - " "use gnulib module copysignf for portability"); # endif #endif #if @GNULIB_COPYSIGN@ # if !@HAVE_COPYSIGN@ _GL_FUNCDECL_SYS (copysign, double, (double x, double y)); # endif _GL_CXXALIAS_SYS (copysign, double, (double x, double y)); _GL_CXXALIASWARN (copysign); #elif defined GNULIB_POSIXCHECK # undef copysign # if HAVE_RAW_DECL_COPYSIGN _GL_WARN_ON_USE (copysign, "copysign is unportable - " "use gnulib module copysign for portability"); # endif #endif #if @GNULIB_COPYSIGNL@ # if !@HAVE_COPYSIGNL@ _GL_FUNCDECL_SYS (copysignl, long double, (long double x, long double y)); # endif _GL_CXXALIAS_SYS (copysignl, long double, (long double x, long double y)); _GL_CXXALIASWARN (copysignl); #elif defined GNULIB_POSIXCHECK # undef copysignl # if HAVE_RAW_DECL_COPYSIGNL _GL_WARN_ON_USE (copysign, "copysignl is unportable - " "use gnulib module copysignl for portability"); # endif #endif #if @GNULIB_COSF@ # if !@HAVE_COSF@ # undef cosf _GL_FUNCDECL_SYS (cosf, float, (float x)); # endif _GL_CXXALIAS_SYS (cosf, float, (float x)); _GL_CXXALIASWARN (cosf); #elif defined GNULIB_POSIXCHECK # undef cosf # if HAVE_RAW_DECL_COSF _GL_WARN_ON_USE (cosf, "cosf is unportable - " "use gnulib module cosf for portability"); # endif #endif #if @GNULIB_COSL@ # if !@HAVE_COSL@ || !@HAVE_DECL_COSL@ # undef cosl _GL_FUNCDECL_SYS (cosl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (cosl, long double, (long double x)); _GL_CXXALIASWARN (cosl); #elif defined GNULIB_POSIXCHECK # undef cosl # if HAVE_RAW_DECL_COSL _GL_WARN_ON_USE (cosl, "cosl is unportable - " "use gnulib module cosl for portability"); # endif #endif #if @GNULIB_COSHF@ # if !@HAVE_COSHF@ # undef coshf _GL_FUNCDECL_SYS (coshf, float, (float x)); # endif _GL_CXXALIAS_SYS (coshf, float, (float x)); _GL_CXXALIASWARN (coshf); #elif defined GNULIB_POSIXCHECK # undef coshf # if HAVE_RAW_DECL_COSHF _GL_WARN_ON_USE (coshf, "coshf is unportable - " "use gnulib module coshf for portability"); # endif #endif #if @GNULIB_EXPF@ # if !@HAVE_EXPF@ # undef expf _GL_FUNCDECL_SYS (expf, float, (float x)); # endif _GL_CXXALIAS_SYS (expf, float, (float x)); _GL_CXXALIASWARN (expf); #elif defined GNULIB_POSIXCHECK # undef expf # if HAVE_RAW_DECL_EXPF _GL_WARN_ON_USE (expf, "expf is unportable - " "use gnulib module expf for portability"); # endif #endif #if @GNULIB_EXPL@ # if !@HAVE_EXPL@ || !@HAVE_DECL_EXPL@ # undef expl _GL_FUNCDECL_SYS (expl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (expl, long double, (long double x)); _GL_CXXALIASWARN (expl); #elif defined GNULIB_POSIXCHECK # undef expl # if HAVE_RAW_DECL_EXPL _GL_WARN_ON_USE (expl, "expl is unportable - " "use gnulib module expl for portability"); # endif #endif #if @GNULIB_EXP2F@ # if !@HAVE_DECL_EXP2F@ _GL_FUNCDECL_SYS (exp2f, float, (float x)); # endif _GL_CXXALIAS_SYS (exp2f, float, (float x)); _GL_CXXALIASWARN (exp2f); #elif defined GNULIB_POSIXCHECK # undef exp2f # if HAVE_RAW_DECL_EXP2F _GL_WARN_ON_USE (exp2f, "exp2f is unportable - " "use gnulib module exp2f for portability"); # endif #endif #if @GNULIB_EXP2@ # if @REPLACE_EXP2@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef exp2 # define exp2 rpl_exp2 # endif _GL_FUNCDECL_RPL (exp2, double, (double x)); _GL_CXXALIAS_RPL (exp2, double, (double x)); # else # if !@HAVE_DECL_EXP2@ _GL_FUNCDECL_SYS (exp2, double, (double x)); # endif _GL_CXXALIAS_SYS (exp2, double, (double x)); # endif _GL_CXXALIASWARN (exp2); #elif defined GNULIB_POSIXCHECK # undef exp2 # if HAVE_RAW_DECL_EXP2 _GL_WARN_ON_USE (exp2, "exp2 is unportable - " "use gnulib module exp2 for portability"); # endif #endif #if @GNULIB_EXP2L@ # if @REPLACE_EXP2L@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef exp2l # define exp2l rpl_exp2l # endif _GL_FUNCDECL_RPL (exp2l, long double, (long double x)); _GL_CXXALIAS_RPL (exp2l, long double, (long double x)); # else # if !@HAVE_DECL_EXP2L@ # undef exp2l _GL_FUNCDECL_SYS (exp2l, long double, (long double x)); # endif _GL_CXXALIAS_SYS (exp2l, long double, (long double x)); # endif _GL_CXXALIASWARN (exp2l); #elif defined GNULIB_POSIXCHECK # undef exp2l # if HAVE_RAW_DECL_EXP2L _GL_WARN_ON_USE (exp2l, "exp2l is unportable - " "use gnulib module exp2l for portability"); # endif #endif #if @GNULIB_EXPM1F@ # if @REPLACE_EXPM1F@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef expm1f # define expm1f rpl_expm1f # endif _GL_FUNCDECL_RPL (expm1f, float, (float x)); _GL_CXXALIAS_RPL (expm1f, float, (float x)); # else # if !@HAVE_EXPM1F@ _GL_FUNCDECL_SYS (expm1f, float, (float x)); # endif _GL_CXXALIAS_SYS (expm1f, float, (float x)); # endif _GL_CXXALIASWARN (expm1f); #elif defined GNULIB_POSIXCHECK # undef expm1f # if HAVE_RAW_DECL_EXPM1F _GL_WARN_ON_USE (expm1f, "expm1f is unportable - " "use gnulib module expm1f for portability"); # endif #endif #if @GNULIB_EXPM1@ # if @REPLACE_EXPM1@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef expm1 # define expm1 rpl_expm1 # endif _GL_FUNCDECL_RPL (expm1, double, (double x)); _GL_CXXALIAS_RPL (expm1, double, (double x)); # else # if !@HAVE_EXPM1@ _GL_FUNCDECL_SYS (expm1, double, (double x)); # endif _GL_CXXALIAS_SYS (expm1, double, (double x)); # endif _GL_CXXALIASWARN (expm1); #elif defined GNULIB_POSIXCHECK # undef expm1 # if HAVE_RAW_DECL_EXPM1 _GL_WARN_ON_USE (expm1, "expm1 is unportable - " "use gnulib module expm1 for portability"); # endif #endif #if @GNULIB_EXPM1L@ # if !@HAVE_DECL_EXPM1L@ # undef expm1l _GL_FUNCDECL_SYS (expm1l, long double, (long double x)); # endif _GL_CXXALIAS_SYS (expm1l, long double, (long double x)); _GL_CXXALIASWARN (expm1l); #elif defined GNULIB_POSIXCHECK # undef expm1l # if HAVE_RAW_DECL_EXPM1L _GL_WARN_ON_USE (expm1l, "expm1l is unportable - " "use gnulib module expm1l for portability"); # endif #endif #if @GNULIB_FABSF@ # if !@HAVE_FABSF@ # undef fabsf _GL_FUNCDECL_SYS (fabsf, float, (float x)); # endif _GL_CXXALIAS_SYS (fabsf, float, (float x)); _GL_CXXALIASWARN (fabsf); #elif defined GNULIB_POSIXCHECK # undef fabsf # if HAVE_RAW_DECL_FABSF _GL_WARN_ON_USE (fabsf, "fabsf is unportable - " "use gnulib module fabsf for portability"); # endif #endif #if @GNULIB_FABSL@ # if @REPLACE_FABSL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fabsl # define fabsl rpl_fabsl # endif _GL_FUNCDECL_RPL (fabsl, long double, (long double x)); _GL_CXXALIAS_RPL (fabsl, long double, (long double x)); # else # if !@HAVE_FABSL@ # undef fabsl _GL_FUNCDECL_SYS (fabsl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (fabsl, long double, (long double x)); # endif _GL_CXXALIASWARN (fabsl); #elif defined GNULIB_POSIXCHECK # undef fabsl # if HAVE_RAW_DECL_FABSL _GL_WARN_ON_USE (fabsl, "fabsl is unportable - " "use gnulib module fabsl for portability"); # endif #endif #if @GNULIB_FLOORF@ # if @REPLACE_FLOORF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef floorf # define floorf rpl_floorf # endif _GL_FUNCDECL_RPL (floorf, float, (float x)); _GL_CXXALIAS_RPL (floorf, float, (float x)); # else # if !@HAVE_DECL_FLOORF@ # undef floorf _GL_FUNCDECL_SYS (floorf, float, (float x)); # endif _GL_CXXALIAS_SYS (floorf, float, (float x)); # endif _GL_CXXALIASWARN (floorf); #elif defined GNULIB_POSIXCHECK # undef floorf # if HAVE_RAW_DECL_FLOORF _GL_WARN_ON_USE (floorf, "floorf is unportable - " "use gnulib module floorf for portability"); # endif #endif #if @GNULIB_FLOOR@ # if @REPLACE_FLOOR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef floor # define floor rpl_floor # endif _GL_FUNCDECL_RPL (floor, double, (double x)); _GL_CXXALIAS_RPL (floor, double, (double x)); # else _GL_CXXALIAS_SYS (floor, double, (double x)); # endif _GL_CXXALIASWARN (floor); #endif #if @GNULIB_FLOORL@ # if @REPLACE_FLOORL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef floorl # define floorl rpl_floorl # endif _GL_FUNCDECL_RPL (floorl, long double, (long double x)); _GL_CXXALIAS_RPL (floorl, long double, (long double x)); # else # if !@HAVE_DECL_FLOORL@ # undef floorl _GL_FUNCDECL_SYS (floorl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (floorl, long double, (long double x)); # endif _GL_CXXALIASWARN (floorl); #elif defined GNULIB_POSIXCHECK # undef floorl # if HAVE_RAW_DECL_FLOORL _GL_WARN_ON_USE (floorl, "floorl is unportable - " "use gnulib module floorl for portability"); # endif #endif #if @GNULIB_FMAF@ # if @REPLACE_FMAF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fmaf # define fmaf rpl_fmaf # endif _GL_FUNCDECL_RPL (fmaf, float, (float x, float y, float z)); _GL_CXXALIAS_RPL (fmaf, float, (float x, float y, float z)); # else # if !@HAVE_FMAF@ _GL_FUNCDECL_SYS (fmaf, float, (float x, float y, float z)); # endif _GL_CXXALIAS_SYS (fmaf, float, (float x, float y, float z)); # endif _GL_CXXALIASWARN (fmaf); #elif defined GNULIB_POSIXCHECK # undef fmaf # if HAVE_RAW_DECL_FMAF _GL_WARN_ON_USE (fmaf, "fmaf is unportable - " "use gnulib module fmaf for portability"); # endif #endif #if @GNULIB_FMA@ # if @REPLACE_FMA@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fma # define fma rpl_fma # endif _GL_FUNCDECL_RPL (fma, double, (double x, double y, double z)); _GL_CXXALIAS_RPL (fma, double, (double x, double y, double z)); # else # if !@HAVE_FMA@ _GL_FUNCDECL_SYS (fma, double, (double x, double y, double z)); # endif _GL_CXXALIAS_SYS (fma, double, (double x, double y, double z)); # endif _GL_CXXALIASWARN (fma); #elif defined GNULIB_POSIXCHECK # undef fma # if HAVE_RAW_DECL_FMA _GL_WARN_ON_USE (fma, "fma is unportable - " "use gnulib module fma for portability"); # endif #endif #if @GNULIB_FMAL@ # if @REPLACE_FMAL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fmal # define fmal rpl_fmal # endif _GL_FUNCDECL_RPL (fmal, long double, (long double x, long double y, long double z)); _GL_CXXALIAS_RPL (fmal, long double, (long double x, long double y, long double z)); # else # if !@HAVE_FMAL@ # undef fmal _GL_FUNCDECL_SYS (fmal, long double, (long double x, long double y, long double z)); # endif _GL_CXXALIAS_SYS (fmal, long double, (long double x, long double y, long double z)); # endif _GL_CXXALIASWARN (fmal); #elif defined GNULIB_POSIXCHECK # undef fmal # if HAVE_RAW_DECL_FMAL _GL_WARN_ON_USE (fmal, "fmal is unportable - " "use gnulib module fmal for portability"); # endif #endif #if @GNULIB_FMODF@ # if @REPLACE_FMODF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fmodf # define fmodf rpl_fmodf # endif _GL_FUNCDECL_RPL (fmodf, float, (float x, float y)); _GL_CXXALIAS_RPL (fmodf, float, (float x, float y)); # else # if !@HAVE_FMODF@ # undef fmodf _GL_FUNCDECL_SYS (fmodf, float, (float x, float y)); # endif _GL_CXXALIAS_SYS (fmodf, float, (float x, float y)); # endif _GL_CXXALIASWARN (fmodf); #elif defined GNULIB_POSIXCHECK # undef fmodf # if HAVE_RAW_DECL_FMODF _GL_WARN_ON_USE (fmodf, "fmodf is unportable - " "use gnulib module fmodf for portability"); # endif #endif #if @GNULIB_FMOD@ # if @REPLACE_FMOD@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fmod # define fmod rpl_fmod # endif _GL_FUNCDECL_RPL (fmod, double, (double x, double y)); _GL_CXXALIAS_RPL (fmod, double, (double x, double y)); # else _GL_CXXALIAS_SYS (fmod, double, (double x, double y)); # endif _GL_CXXALIASWARN (fmod); #elif defined GNULIB_POSIXCHECK # undef fmod # if HAVE_RAW_DECL_FMOD _GL_WARN_ON_USE (fmod, "fmod has portability problems - " "use gnulib module fmod for portability"); # endif #endif #if @GNULIB_FMODL@ # if @REPLACE_FMODL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fmodl # define fmodl rpl_fmodl # endif _GL_FUNCDECL_RPL (fmodl, long double, (long double x, long double y)); _GL_CXXALIAS_RPL (fmodl, long double, (long double x, long double y)); # else # if !@HAVE_FMODL@ # undef fmodl _GL_FUNCDECL_SYS (fmodl, long double, (long double x, long double y)); # endif _GL_CXXALIAS_SYS (fmodl, long double, (long double x, long double y)); # endif _GL_CXXALIASWARN (fmodl); #elif defined GNULIB_POSIXCHECK # undef fmodl # if HAVE_RAW_DECL_FMODL _GL_WARN_ON_USE (fmodl, "fmodl is unportable - " "use gnulib module fmodl for portability"); # endif #endif /* Write x as x = mantissa * 2^exp where If x finite and nonzero: 0.5 <= |mantissa| < 1.0. If x is zero: mantissa = x, exp = 0. If x is infinite or NaN: mantissa = x, exp unspecified. Store exp in *EXPPTR and return mantissa. */ #if @GNULIB_FREXPF@ # if @REPLACE_FREXPF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef frexpf # define frexpf rpl_frexpf # endif _GL_FUNCDECL_RPL (frexpf, float, (float x, int *expptr) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (frexpf, float, (float x, int *expptr)); # else # if !@HAVE_FREXPF@ # undef frexpf _GL_FUNCDECL_SYS (frexpf, float, (float x, int *expptr) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (frexpf, float, (float x, int *expptr)); # endif _GL_CXXALIASWARN (frexpf); #elif defined GNULIB_POSIXCHECK # undef frexpf # if HAVE_RAW_DECL_FREXPF _GL_WARN_ON_USE (frexpf, "frexpf is unportable - " "use gnulib module frexpf for portability"); # endif #endif /* Write x as x = mantissa * 2^exp where If x finite and nonzero: 0.5 <= |mantissa| < 1.0. If x is zero: mantissa = x, exp = 0. If x is infinite or NaN: mantissa = x, exp unspecified. Store exp in *EXPPTR and return mantissa. */ #if @GNULIB_FREXP@ # if @REPLACE_FREXP@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef frexp # define frexp rpl_frexp # endif _GL_FUNCDECL_RPL (frexp, double, (double x, int *expptr) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (frexp, double, (double x, int *expptr)); # else _GL_CXXALIAS_SYS (frexp, double, (double x, int *expptr)); # endif _GL_CXXALIASWARN (frexp); #elif defined GNULIB_POSIXCHECK # undef frexp /* Assume frexp is always declared. */ _GL_WARN_ON_USE (frexp, "frexp is unportable - " "use gnulib module frexp for portability"); #endif /* Write x as x = mantissa * 2^exp where If x finite and nonzero: 0.5 <= |mantissa| < 1.0. If x is zero: mantissa = x, exp = 0. If x is infinite or NaN: mantissa = x, exp unspecified. Store exp in *EXPPTR and return mantissa. */ #if @GNULIB_FREXPL@ && @REPLACE_FREXPL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef frexpl # define frexpl rpl_frexpl # endif _GL_FUNCDECL_RPL (frexpl, long double, (long double x, int *expptr) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (frexpl, long double, (long double x, int *expptr)); #else # if !@HAVE_DECL_FREXPL@ _GL_FUNCDECL_SYS (frexpl, long double, (long double x, int *expptr) _GL_ARG_NONNULL ((2))); # endif # if @GNULIB_FREXPL@ _GL_CXXALIAS_SYS (frexpl, long double, (long double x, int *expptr)); # endif #endif #if @GNULIB_FREXPL@ && !(@REPLACE_FREXPL@ && !@HAVE_DECL_FREXPL@) _GL_CXXALIASWARN (frexpl); #endif #if !@GNULIB_FREXPL@ && defined GNULIB_POSIXCHECK # undef frexpl # if HAVE_RAW_DECL_FREXPL _GL_WARN_ON_USE (frexpl, "frexpl is unportable - " "use gnulib module frexpl for portability"); # endif #endif /* Return sqrt(x^2+y^2). */ #if @GNULIB_HYPOTF@ # if @REPLACE_HYPOTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef hypotf # define hypotf rpl_hypotf # endif _GL_FUNCDECL_RPL (hypotf, float, (float x, float y)); _GL_CXXALIAS_RPL (hypotf, float, (float x, float y)); # else # if !@HAVE_HYPOTF@ _GL_FUNCDECL_SYS (hypotf, float, (float x, float y)); # endif _GL_CXXALIAS_SYS (hypotf, float, (float x, float y)); # endif _GL_CXXALIASWARN (hypotf); #elif defined GNULIB_POSIXCHECK # undef hypotf # if HAVE_RAW_DECL_HYPOTF _GL_WARN_ON_USE (hypotf, "hypotf is unportable - " "use gnulib module hypotf for portability"); # endif #endif /* Return sqrt(x^2+y^2). */ #if @GNULIB_HYPOT@ # if @REPLACE_HYPOT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef hypot # define hypot rpl_hypot # endif _GL_FUNCDECL_RPL (hypot, double, (double x, double y)); _GL_CXXALIAS_RPL (hypot, double, (double x, double y)); # else _GL_CXXALIAS_SYS (hypot, double, (double x, double y)); # endif _GL_CXXALIASWARN (hypot); #elif defined GNULIB_POSIXCHECK # undef hypot # if HAVE_RAW_DECL_HYPOT _GL_WARN_ON_USE (hypotf, "hypot has portability problems - " "use gnulib module hypot for portability"); # endif #endif /* Return sqrt(x^2+y^2). */ #if @GNULIB_HYPOTL@ # if @REPLACE_HYPOTL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef hypotl # define hypotl rpl_hypotl # endif _GL_FUNCDECL_RPL (hypotl, long double, (long double x, long double y)); _GL_CXXALIAS_RPL (hypotl, long double, (long double x, long double y)); # else # if !@HAVE_HYPOTL@ _GL_FUNCDECL_SYS (hypotl, long double, (long double x, long double y)); # endif _GL_CXXALIAS_SYS (hypotl, long double, (long double x, long double y)); # endif _GL_CXXALIASWARN (hypotl); #elif defined GNULIB_POSIXCHECK # undef hypotl # if HAVE_RAW_DECL_HYPOTL _GL_WARN_ON_USE (hypotl, "hypotl is unportable - " "use gnulib module hypotl for portability"); # endif #endif #if @GNULIB_ILOGBF@ # if @REPLACE_ILOGBF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ilogbf # define ilogbf rpl_ilogbf # endif _GL_FUNCDECL_RPL (ilogbf, int, (float x)); _GL_CXXALIAS_RPL (ilogbf, int, (float x)); # else # if !@HAVE_ILOGBF@ _GL_FUNCDECL_SYS (ilogbf, int, (float x)); # endif _GL_CXXALIAS_SYS (ilogbf, int, (float x)); # endif _GL_CXXALIASWARN (ilogbf); #elif defined GNULIB_POSIXCHECK # undef ilogbf # if HAVE_RAW_DECL_ILOGBF _GL_WARN_ON_USE (ilogbf, "ilogbf is unportable - " "use gnulib module ilogbf for portability"); # endif #endif #if @GNULIB_ILOGB@ # if @REPLACE_ILOGB@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ilogb # define ilogb rpl_ilogb # endif _GL_FUNCDECL_RPL (ilogb, int, (double x)); _GL_CXXALIAS_RPL (ilogb, int, (double x)); # else # if !@HAVE_ILOGB@ _GL_FUNCDECL_SYS (ilogb, int, (double x)); # endif _GL_CXXALIAS_SYS (ilogb, int, (double x)); # endif _GL_CXXALIASWARN (ilogb); #elif defined GNULIB_POSIXCHECK # undef ilogb # if HAVE_RAW_DECL_ILOGB _GL_WARN_ON_USE (ilogb, "ilogb is unportable - " "use gnulib module ilogb for portability"); # endif #endif #if @GNULIB_ILOGBL@ # if !@HAVE_ILOGBL@ _GL_FUNCDECL_SYS (ilogbl, int, (long double x)); # endif _GL_CXXALIAS_SYS (ilogbl, int, (long double x)); _GL_CXXALIASWARN (ilogbl); #elif defined GNULIB_POSIXCHECK # undef ilogbl # if HAVE_RAW_DECL_ILOGBL _GL_WARN_ON_USE (ilogbl, "ilogbl is unportable - " "use gnulib module ilogbl for portability"); # endif #endif /* Return x * 2^exp. */ #if @GNULIB_LDEXPF@ # if !@HAVE_LDEXPF@ # undef ldexpf _GL_FUNCDECL_SYS (ldexpf, float, (float x, int exp)); # endif _GL_CXXALIAS_SYS (ldexpf, float, (float x, int exp)); _GL_CXXALIASWARN (ldexpf); #elif defined GNULIB_POSIXCHECK # undef ldexpf # if HAVE_RAW_DECL_LDEXPF _GL_WARN_ON_USE (ldexpf, "ldexpf is unportable - " "use gnulib module ldexpf for portability"); # endif #endif /* Return x * 2^exp. */ #if @GNULIB_LDEXPL@ && @REPLACE_LDEXPL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ldexpl # define ldexpl rpl_ldexpl # endif _GL_FUNCDECL_RPL (ldexpl, long double, (long double x, int exp)); _GL_CXXALIAS_RPL (ldexpl, long double, (long double x, int exp)); #else # if !@HAVE_DECL_LDEXPL@ _GL_FUNCDECL_SYS (ldexpl, long double, (long double x, int exp)); # endif # if @GNULIB_LDEXPL@ _GL_CXXALIAS_SYS (ldexpl, long double, (long double x, int exp)); # endif #endif #if @GNULIB_LDEXPL@ _GL_CXXALIASWARN (ldexpl); #endif #if !@GNULIB_LDEXPL@ && defined GNULIB_POSIXCHECK # undef ldexpl # if HAVE_RAW_DECL_LDEXPL _GL_WARN_ON_USE (ldexpl, "ldexpl is unportable - " "use gnulib module ldexpl for portability"); # endif #endif #if @GNULIB_LOGF@ # if @REPLACE_LOGF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef logf # define logf rpl_logf # endif _GL_FUNCDECL_RPL (logf, float, (float x)); _GL_CXXALIAS_RPL (logf, float, (float x)); # else # if !@HAVE_LOGF@ # undef logf _GL_FUNCDECL_SYS (logf, float, (float x)); # endif _GL_CXXALIAS_SYS (logf, float, (float x)); # endif _GL_CXXALIASWARN (logf); #elif defined GNULIB_POSIXCHECK # undef logf # if HAVE_RAW_DECL_LOGF _GL_WARN_ON_USE (logf, "logf is unportable - " "use gnulib module logf for portability"); # endif #endif #if @GNULIB_LOG@ # if @REPLACE_LOG@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log # define log rpl_log # endif _GL_FUNCDECL_RPL (log, double, (double x)); _GL_CXXALIAS_RPL (log, double, (double x)); # else _GL_CXXALIAS_SYS (log, double, (double x)); # endif _GL_CXXALIASWARN (log); #elif defined GNULIB_POSIXCHECK # undef log # if HAVE_RAW_DECL_LOG _GL_WARN_ON_USE (log, "log has portability problems - " "use gnulib module log for portability"); # endif #endif #if @GNULIB_LOGL@ # if @REPLACE_LOGL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef logl # define logl rpl_logl # endif _GL_FUNCDECL_RPL (logl, long double, (long double x)); _GL_CXXALIAS_RPL (logl, long double, (long double x)); # else # if !@HAVE_LOGL@ || !@HAVE_DECL_LOGL@ # undef logl _GL_FUNCDECL_SYS (logl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (logl, long double, (long double x)); # endif _GL_CXXALIASWARN (logl); #elif defined GNULIB_POSIXCHECK # undef logl # if HAVE_RAW_DECL_LOGL _GL_WARN_ON_USE (logl, "logl is unportable - " "use gnulib module logl for portability"); # endif #endif #if @GNULIB_LOG10F@ # if @REPLACE_LOG10F@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log10f # define log10f rpl_log10f # endif _GL_FUNCDECL_RPL (log10f, float, (float x)); _GL_CXXALIAS_RPL (log10f, float, (float x)); # else # if !@HAVE_LOG10F@ # undef log10f _GL_FUNCDECL_SYS (log10f, float, (float x)); # endif _GL_CXXALIAS_SYS (log10f, float, (float x)); # endif _GL_CXXALIASWARN (log10f); #elif defined GNULIB_POSIXCHECK # undef log10f # if HAVE_RAW_DECL_LOG10F _GL_WARN_ON_USE (log10f, "log10f is unportable - " "use gnulib module log10f for portability"); # endif #endif #if @GNULIB_LOG10@ # if @REPLACE_LOG10@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log10 # define log10 rpl_log10 # endif _GL_FUNCDECL_RPL (log10, double, (double x)); _GL_CXXALIAS_RPL (log10, double, (double x)); # else _GL_CXXALIAS_SYS (log10, double, (double x)); # endif _GL_CXXALIASWARN (log10); #elif defined GNULIB_POSIXCHECK # undef log10 # if HAVE_RAW_DECL_LOG10 _GL_WARN_ON_USE (log10, "log10 has portability problems - " "use gnulib module log10 for portability"); # endif #endif #if @GNULIB_LOG10L@ # if @REPLACE_LOG10L@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log10l # define log10l rpl_log10l # endif _GL_FUNCDECL_RPL (log10l, long double, (long double x)); _GL_CXXALIAS_RPL (log10l, long double, (long double x)); # else # if !@HAVE_LOG10L@ || !@HAVE_DECL_LOG10L@ # undef log10l _GL_FUNCDECL_SYS (log10l, long double, (long double x)); # endif _GL_CXXALIAS_SYS (log10l, long double, (long double x)); # endif _GL_CXXALIASWARN (log10l); #elif defined GNULIB_POSIXCHECK # undef log10l # if HAVE_RAW_DECL_LOG10L _GL_WARN_ON_USE (log10l, "log10l is unportable - " "use gnulib module log10l for portability"); # endif #endif #if @GNULIB_LOG1PF@ # if @REPLACE_LOG1PF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log1pf # define log1pf rpl_log1pf # endif _GL_FUNCDECL_RPL (log1pf, float, (float x)); _GL_CXXALIAS_RPL (log1pf, float, (float x)); # else # if !@HAVE_LOG1PF@ _GL_FUNCDECL_SYS (log1pf, float, (float x)); # endif _GL_CXXALIAS_SYS (log1pf, float, (float x)); # endif _GL_CXXALIASWARN (log1pf); #elif defined GNULIB_POSIXCHECK # undef log1pf # if HAVE_RAW_DECL_LOG1PF _GL_WARN_ON_USE (log1pf, "log1pf is unportable - " "use gnulib module log1pf for portability"); # endif #endif #if @GNULIB_LOG1P@ # if @REPLACE_LOG1P@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log1p # define log1p rpl_log1p # endif _GL_FUNCDECL_RPL (log1p, double, (double x)); _GL_CXXALIAS_RPL (log1p, double, (double x)); # else # if !@HAVE_LOG1P@ _GL_FUNCDECL_SYS (log1p, double, (double x)); # endif _GL_CXXALIAS_SYS (log1p, double, (double x)); # endif _GL_CXXALIASWARN (log1p); #elif defined GNULIB_POSIXCHECK # undef log1p # if HAVE_RAW_DECL_LOG1P _GL_WARN_ON_USE (log1p, "log1p has portability problems - " "use gnulib module log1p for portability"); # endif #endif #if @GNULIB_LOG1PL@ # if @REPLACE_LOG1PL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log1pl # define log1pl rpl_log1pl # endif _GL_FUNCDECL_RPL (log1pl, long double, (long double x)); _GL_CXXALIAS_RPL (log1pl, long double, (long double x)); # else # if !@HAVE_LOG1PL@ _GL_FUNCDECL_SYS (log1pl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (log1pl, long double, (long double x)); # endif _GL_CXXALIASWARN (log1pl); #elif defined GNULIB_POSIXCHECK # undef log1pl # if HAVE_RAW_DECL_LOG1PL _GL_WARN_ON_USE (log1pl, "log1pl has portability problems - " "use gnulib module log1pl for portability"); # endif #endif #if @GNULIB_LOG2F@ # if @REPLACE_LOG2F@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log2f # define log2f rpl_log2f # endif _GL_FUNCDECL_RPL (log2f, float, (float x)); _GL_CXXALIAS_RPL (log2f, float, (float x)); # else # if !@HAVE_DECL_LOG2F@ # undef log2f _GL_FUNCDECL_SYS (log2f, float, (float x)); # endif _GL_CXXALIAS_SYS (log2f, float, (float x)); # endif _GL_CXXALIASWARN (log2f); #elif defined GNULIB_POSIXCHECK # undef log2f # if HAVE_RAW_DECL_LOG2F _GL_WARN_ON_USE (log2f, "log2f is unportable - " "use gnulib module log2f for portability"); # endif #endif #if @GNULIB_LOG2@ # if @REPLACE_LOG2@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log2 # define log2 rpl_log2 # endif _GL_FUNCDECL_RPL (log2, double, (double x)); _GL_CXXALIAS_RPL (log2, double, (double x)); # else # if !@HAVE_DECL_LOG2@ # undef log2 _GL_FUNCDECL_SYS (log2, double, (double x)); # endif _GL_CXXALIAS_SYS (log2, double, (double x)); # endif _GL_CXXALIASWARN (log2); #elif defined GNULIB_POSIXCHECK # undef log2 # if HAVE_RAW_DECL_LOG2 _GL_WARN_ON_USE (log2, "log2 is unportable - " "use gnulib module log2 for portability"); # endif #endif #if @GNULIB_LOG2L@ # if @REPLACE_LOG2L@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log2l # define log2l rpl_log2l # endif _GL_FUNCDECL_RPL (log2l, long double, (long double x)); _GL_CXXALIAS_RPL (log2l, long double, (long double x)); # else # if !@HAVE_DECL_LOG2L@ _GL_FUNCDECL_SYS (log2l, long double, (long double x)); # endif _GL_CXXALIAS_SYS (log2l, long double, (long double x)); # endif _GL_CXXALIASWARN (log2l); #elif defined GNULIB_POSIXCHECK # undef log2l # if HAVE_RAW_DECL_LOG2L _GL_WARN_ON_USE (log2l, "log2l is unportable - " "use gnulib module log2l for portability"); # endif #endif #if @GNULIB_LOGBF@ # if @REPLACE_LOGBF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef logbf # define logbf rpl_logbf # endif _GL_FUNCDECL_RPL (logbf, float, (float x)); _GL_CXXALIAS_RPL (logbf, float, (float x)); # else # if !@HAVE_LOGBF@ _GL_FUNCDECL_SYS (logbf, float, (float x)); # endif _GL_CXXALIAS_SYS (logbf, float, (float x)); # endif _GL_CXXALIASWARN (logbf); #elif defined GNULIB_POSIXCHECK # undef logbf # if HAVE_RAW_DECL_LOGBF _GL_WARN_ON_USE (logbf, "logbf is unportable - " "use gnulib module logbf for portability"); # endif #endif #if @GNULIB_LOGB@ # if @REPLACE_LOGB@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef logb # define logb rpl_logb # endif _GL_FUNCDECL_RPL (logb, double, (double x)); _GL_CXXALIAS_RPL (logb, double, (double x)); # else # if !@HAVE_DECL_LOGB@ _GL_FUNCDECL_SYS (logb, double, (double x)); # endif _GL_CXXALIAS_SYS (logb, double, (double x)); # endif _GL_CXXALIASWARN (logb); #elif defined GNULIB_POSIXCHECK # undef logb # if HAVE_RAW_DECL_LOGB _GL_WARN_ON_USE (logb, "logb is unportable - " "use gnulib module logb for portability"); # endif #endif #if @GNULIB_LOGBL@ # if @REPLACE_LOGBL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef logbl # define logbl rpl_logbl # endif _GL_FUNCDECL_RPL (logbl, long double, (long double x)); _GL_CXXALIAS_RPL (logbl, long double, (long double x)); # else # if !@HAVE_LOGBL@ _GL_FUNCDECL_SYS (logbl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (logbl, long double, (long double x)); # endif _GL_CXXALIASWARN (logbl); #elif defined GNULIB_POSIXCHECK # undef logbl # if HAVE_RAW_DECL_LOGBL _GL_WARN_ON_USE (logbl, "logbl is unportable - " "use gnulib module logbl for portability"); # endif #endif #if @GNULIB_MODFF@ # if @REPLACE_MODFF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef modff # define modff rpl_modff # endif _GL_FUNCDECL_RPL (modff, float, (float x, float *iptr) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (modff, float, (float x, float *iptr)); # else # if !@HAVE_MODFF@ # undef modff _GL_FUNCDECL_SYS (modff, float, (float x, float *iptr) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (modff, float, (float x, float *iptr)); # endif _GL_CXXALIASWARN (modff); #elif defined GNULIB_POSIXCHECK # undef modff # if HAVE_RAW_DECL_MODFF _GL_WARN_ON_USE (modff, "modff is unportable - " "use gnulib module modff for portability"); # endif #endif #if @GNULIB_MODF@ # if @REPLACE_MODF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef modf # define modf rpl_modf # endif _GL_FUNCDECL_RPL (modf, double, (double x, double *iptr) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (modf, double, (double x, double *iptr)); # else _GL_CXXALIAS_SYS (modf, double, (double x, double *iptr)); # endif _GL_CXXALIASWARN (modf); #elif defined GNULIB_POSIXCHECK # undef modf # if HAVE_RAW_DECL_MODF _GL_WARN_ON_USE (modf, "modf has portability problems - " "use gnulib module modf for portability"); # endif #endif #if @GNULIB_MODFL@ # if @REPLACE_MODFL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef modfl # define modfl rpl_modfl # endif _GL_FUNCDECL_RPL (modfl, long double, (long double x, long double *iptr) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (modfl, long double, (long double x, long double *iptr)); # else # if !@HAVE_MODFL@ # undef modfl _GL_FUNCDECL_SYS (modfl, long double, (long double x, long double *iptr) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (modfl, long double, (long double x, long double *iptr)); # endif _GL_CXXALIASWARN (modfl); #elif defined GNULIB_POSIXCHECK # undef modfl # if HAVE_RAW_DECL_MODFL _GL_WARN_ON_USE (modfl, "modfl is unportable - " "use gnulib module modfl for portability"); # endif #endif #if @GNULIB_POWF@ # if !@HAVE_POWF@ # undef powf _GL_FUNCDECL_SYS (powf, float, (float x, float y)); # endif _GL_CXXALIAS_SYS (powf, float, (float x, float y)); _GL_CXXALIASWARN (powf); #elif defined GNULIB_POSIXCHECK # undef powf # if HAVE_RAW_DECL_POWF _GL_WARN_ON_USE (powf, "powf is unportable - " "use gnulib module powf for portability"); # endif #endif #if @GNULIB_REMAINDERF@ # if @REPLACE_REMAINDERF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef remainderf # define remainderf rpl_remainderf # endif _GL_FUNCDECL_RPL (remainderf, float, (float x, float y)); _GL_CXXALIAS_RPL (remainderf, float, (float x, float y)); # else # if !@HAVE_REMAINDERF@ _GL_FUNCDECL_SYS (remainderf, float, (float x, float y)); # endif _GL_CXXALIAS_SYS (remainderf, float, (float x, float y)); # endif _GL_CXXALIASWARN (remainderf); #elif defined GNULIB_POSIXCHECK # undef remainderf # if HAVE_RAW_DECL_REMAINDERF _GL_WARN_ON_USE (remainderf, "remainderf is unportable - " "use gnulib module remainderf for portability"); # endif #endif #if @GNULIB_REMAINDER@ # if @REPLACE_REMAINDER@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef remainder # define remainder rpl_remainder # endif _GL_FUNCDECL_RPL (remainder, double, (double x, double y)); _GL_CXXALIAS_RPL (remainder, double, (double x, double y)); # else # if !@HAVE_REMAINDER@ || !@HAVE_DECL_REMAINDER@ _GL_FUNCDECL_SYS (remainder, double, (double x, double y)); # endif _GL_CXXALIAS_SYS (remainder, double, (double x, double y)); # endif _GL_CXXALIASWARN (remainder); #elif defined GNULIB_POSIXCHECK # undef remainder # if HAVE_RAW_DECL_REMAINDER _GL_WARN_ON_USE (remainder, "remainder is unportable - " "use gnulib module remainder for portability"); # endif #endif #if @GNULIB_REMAINDERL@ # if @REPLACE_REMAINDERL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef remainderl # define remainderl rpl_remainderl # endif _GL_FUNCDECL_RPL (remainderl, long double, (long double x, long double y)); _GL_CXXALIAS_RPL (remainderl, long double, (long double x, long double y)); # else # if !@HAVE_DECL_REMAINDERL@ # undef remainderl _GL_FUNCDECL_SYS (remainderl, long double, (long double x, long double y)); # endif _GL_CXXALIAS_SYS (remainderl, long double, (long double x, long double y)); # endif _GL_CXXALIASWARN (remainderl); #elif defined GNULIB_POSIXCHECK # undef remainderl # if HAVE_RAW_DECL_REMAINDERL _GL_WARN_ON_USE (remainderl, "remainderl is unportable - " "use gnulib module remainderl for portability"); # endif #endif #if @GNULIB_RINTF@ # if !@HAVE_DECL_RINTF@ _GL_FUNCDECL_SYS (rintf, float, (float x)); # endif _GL_CXXALIAS_SYS (rintf, float, (float x)); _GL_CXXALIASWARN (rintf); #elif defined GNULIB_POSIXCHECK # undef rintf # if HAVE_RAW_DECL_RINTF _GL_WARN_ON_USE (rintf, "rintf is unportable - " "use gnulib module rintf for portability"); # endif #endif #if @GNULIB_RINT@ # if !@HAVE_RINT@ _GL_FUNCDECL_SYS (rint, double, (double x)); # endif _GL_CXXALIAS_SYS (rint, double, (double x)); _GL_CXXALIASWARN (rint); #elif defined GNULIB_POSIXCHECK # undef rint # if HAVE_RAW_DECL_RINT _GL_WARN_ON_USE (rint, "rint is unportable - " "use gnulib module rint for portability"); # endif #endif #if @GNULIB_RINTL@ # if !@HAVE_RINTL@ _GL_FUNCDECL_SYS (rintl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (rintl, long double, (long double x)); _GL_CXXALIASWARN (rintl); #elif defined GNULIB_POSIXCHECK # undef rintl # if HAVE_RAW_DECL_RINTL _GL_WARN_ON_USE (rintl, "rintl is unportable - " "use gnulib module rintl for portability"); # endif #endif #if @GNULIB_ROUNDF@ # if @REPLACE_ROUNDF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef roundf # define roundf rpl_roundf # endif _GL_FUNCDECL_RPL (roundf, float, (float x)); _GL_CXXALIAS_RPL (roundf, float, (float x)); # else # if !@HAVE_DECL_ROUNDF@ _GL_FUNCDECL_SYS (roundf, float, (float x)); # endif _GL_CXXALIAS_SYS (roundf, float, (float x)); # endif _GL_CXXALIASWARN (roundf); #elif defined GNULIB_POSIXCHECK # undef roundf # if HAVE_RAW_DECL_ROUNDF _GL_WARN_ON_USE (roundf, "roundf is unportable - " "use gnulib module roundf for portability"); # endif #endif #if @GNULIB_ROUND@ # if @REPLACE_ROUND@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef round # define round rpl_round # endif _GL_FUNCDECL_RPL (round, double, (double x)); _GL_CXXALIAS_RPL (round, double, (double x)); # else # if !@HAVE_DECL_ROUND@ _GL_FUNCDECL_SYS (round, double, (double x)); # endif _GL_CXXALIAS_SYS (round, double, (double x)); # endif _GL_CXXALIASWARN (round); #elif defined GNULIB_POSIXCHECK # undef round # if HAVE_RAW_DECL_ROUND _GL_WARN_ON_USE (round, "round is unportable - " "use gnulib module round for portability"); # endif #endif #if @GNULIB_ROUNDL@ # if @REPLACE_ROUNDL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef roundl # define roundl rpl_roundl # endif _GL_FUNCDECL_RPL (roundl, long double, (long double x)); _GL_CXXALIAS_RPL (roundl, long double, (long double x)); # else # if !@HAVE_DECL_ROUNDL@ # undef roundl _GL_FUNCDECL_SYS (roundl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (roundl, long double, (long double x)); # endif _GL_CXXALIASWARN (roundl); #elif defined GNULIB_POSIXCHECK # undef roundl # if HAVE_RAW_DECL_ROUNDL _GL_WARN_ON_USE (roundl, "roundl is unportable - " "use gnulib module roundl for portability"); # endif #endif #if @GNULIB_SINF@ # if !@HAVE_SINF@ # undef sinf _GL_FUNCDECL_SYS (sinf, float, (float x)); # endif _GL_CXXALIAS_SYS (sinf, float, (float x)); _GL_CXXALIASWARN (sinf); #elif defined GNULIB_POSIXCHECK # undef sinf # if HAVE_RAW_DECL_SINF _GL_WARN_ON_USE (sinf, "sinf is unportable - " "use gnulib module sinf for portability"); # endif #endif #if @GNULIB_SINL@ # if !@HAVE_SINL@ || !@HAVE_DECL_SINL@ # undef sinl _GL_FUNCDECL_SYS (sinl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (sinl, long double, (long double x)); _GL_CXXALIASWARN (sinl); #elif defined GNULIB_POSIXCHECK # undef sinl # if HAVE_RAW_DECL_SINL _GL_WARN_ON_USE (sinl, "sinl is unportable - " "use gnulib module sinl for portability"); # endif #endif #if @GNULIB_SINHF@ # if !@HAVE_SINHF@ # undef sinhf _GL_FUNCDECL_SYS (sinhf, float, (float x)); # endif _GL_CXXALIAS_SYS (sinhf, float, (float x)); _GL_CXXALIASWARN (sinhf); #elif defined GNULIB_POSIXCHECK # undef sinhf # if HAVE_RAW_DECL_SINHF _GL_WARN_ON_USE (sinhf, "sinhf is unportable - " "use gnulib module sinhf for portability"); # endif #endif #if @GNULIB_SQRTF@ # if !@HAVE_SQRTF@ # undef sqrtf _GL_FUNCDECL_SYS (sqrtf, float, (float x)); # endif _GL_CXXALIAS_SYS (sqrtf, float, (float x)); _GL_CXXALIASWARN (sqrtf); #elif defined GNULIB_POSIXCHECK # undef sqrtf # if HAVE_RAW_DECL_SQRTF _GL_WARN_ON_USE (sqrtf, "sqrtf is unportable - " "use gnulib module sqrtf for portability"); # endif #endif #if @GNULIB_SQRTL@ # if @REPLACE_SQRTL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef sqrtl # define sqrtl rpl_sqrtl # endif _GL_FUNCDECL_RPL (sqrtl, long double, (long double x)); _GL_CXXALIAS_RPL (sqrtl, long double, (long double x)); # else # if !@HAVE_SQRTL@ || !@HAVE_DECL_SQRTL@ # undef sqrtl _GL_FUNCDECL_SYS (sqrtl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (sqrtl, long double, (long double x)); # endif _GL_CXXALIASWARN (sqrtl); #elif defined GNULIB_POSIXCHECK # undef sqrtl # if HAVE_RAW_DECL_SQRTL _GL_WARN_ON_USE (sqrtl, "sqrtl is unportable - " "use gnulib module sqrtl for portability"); # endif #endif #if @GNULIB_TANF@ # if !@HAVE_TANF@ # undef tanf _GL_FUNCDECL_SYS (tanf, float, (float x)); # endif _GL_CXXALIAS_SYS (tanf, float, (float x)); _GL_CXXALIASWARN (tanf); #elif defined GNULIB_POSIXCHECK # undef tanf # if HAVE_RAW_DECL_TANF _GL_WARN_ON_USE (tanf, "tanf is unportable - " "use gnulib module tanf for portability"); # endif #endif #if @GNULIB_TANL@ # if !@HAVE_TANL@ || !@HAVE_DECL_TANL@ # undef tanl _GL_FUNCDECL_SYS (tanl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (tanl, long double, (long double x)); _GL_CXXALIASWARN (tanl); #elif defined GNULIB_POSIXCHECK # undef tanl # if HAVE_RAW_DECL_TANL _GL_WARN_ON_USE (tanl, "tanl is unportable - " "use gnulib module tanl for portability"); # endif #endif #if @GNULIB_TANHF@ # if !@HAVE_TANHF@ # undef tanhf _GL_FUNCDECL_SYS (tanhf, float, (float x)); # endif _GL_CXXALIAS_SYS (tanhf, float, (float x)); _GL_CXXALIASWARN (tanhf); #elif defined GNULIB_POSIXCHECK # undef tanhf # if HAVE_RAW_DECL_TANHF _GL_WARN_ON_USE (tanhf, "tanhf is unportable - " "use gnulib module tanhf for portability"); # endif #endif #if @GNULIB_TRUNCF@ # if @REPLACE_TRUNCF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef truncf # define truncf rpl_truncf # endif _GL_FUNCDECL_RPL (truncf, float, (float x)); _GL_CXXALIAS_RPL (truncf, float, (float x)); # else # if !@HAVE_DECL_TRUNCF@ _GL_FUNCDECL_SYS (truncf, float, (float x)); # endif _GL_CXXALIAS_SYS (truncf, float, (float x)); # endif _GL_CXXALIASWARN (truncf); #elif defined GNULIB_POSIXCHECK # undef truncf # if HAVE_RAW_DECL_TRUNCF _GL_WARN_ON_USE (truncf, "truncf is unportable - " "use gnulib module truncf for portability"); # endif #endif #if @GNULIB_TRUNC@ # if @REPLACE_TRUNC@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef trunc # define trunc rpl_trunc # endif _GL_FUNCDECL_RPL (trunc, double, (double x)); _GL_CXXALIAS_RPL (trunc, double, (double x)); # else # if !@HAVE_DECL_TRUNC@ _GL_FUNCDECL_SYS (trunc, double, (double x)); # endif _GL_CXXALIAS_SYS (trunc, double, (double x)); # endif _GL_CXXALIASWARN (trunc); #elif defined GNULIB_POSIXCHECK # undef trunc # if HAVE_RAW_DECL_TRUNC _GL_WARN_ON_USE (trunc, "trunc is unportable - " "use gnulib module trunc for portability"); # endif #endif #if @GNULIB_TRUNCL@ # if @REPLACE_TRUNCL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef truncl # define truncl rpl_truncl # endif _GL_FUNCDECL_RPL (truncl, long double, (long double x)); _GL_CXXALIAS_RPL (truncl, long double, (long double x)); # else # if !@HAVE_DECL_TRUNCL@ _GL_FUNCDECL_SYS (truncl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (truncl, long double, (long double x)); # endif _GL_CXXALIASWARN (truncl); #elif defined GNULIB_POSIXCHECK # undef truncl # if HAVE_RAW_DECL_TRUNCL _GL_WARN_ON_USE (truncl, "truncl is unportable - " "use gnulib module truncl for portability"); # endif #endif /* Definitions of function-like macros come here, after the function declarations. */ #if @GNULIB_ISFINITE@ # if @REPLACE_ISFINITE@ _GL_EXTERN_C int gl_isfinitef (float x); _GL_EXTERN_C int gl_isfinited (double x); _GL_EXTERN_C int gl_isfinitel (long double x); # undef isfinite # define isfinite(x) \ (sizeof (x) == sizeof (long double) ? gl_isfinitel (x) : \ sizeof (x) == sizeof (double) ? gl_isfinited (x) : \ gl_isfinitef (x)) # endif # ifdef __cplusplus # ifdef isfinite _GL_MATH_CXX_REAL_FLOATING_DECL_1 (isfinite) # undef isfinite _GL_MATH_CXX_REAL_FLOATING_DECL_2 (isfinite) # endif # endif #elif defined GNULIB_POSIXCHECK # if defined isfinite _GL_WARN_REAL_FLOATING_DECL (isfinite); # undef isfinite # define isfinite(x) _GL_WARN_REAL_FLOATING_IMPL (isfinite, x) # endif #endif #if @GNULIB_ISINF@ # if @REPLACE_ISINF@ _GL_EXTERN_C int gl_isinff (float x); _GL_EXTERN_C int gl_isinfd (double x); _GL_EXTERN_C int gl_isinfl (long double x); # undef isinf # define isinf(x) \ (sizeof (x) == sizeof (long double) ? gl_isinfl (x) : \ sizeof (x) == sizeof (double) ? gl_isinfd (x) : \ gl_isinff (x)) # endif # ifdef __cplusplus # ifdef isinf _GL_MATH_CXX_REAL_FLOATING_DECL_1 (isinf) # undef isinf _GL_MATH_CXX_REAL_FLOATING_DECL_2 (isinf) # endif # endif #elif defined GNULIB_POSIXCHECK # if defined isinf _GL_WARN_REAL_FLOATING_DECL (isinf); # undef isinf # define isinf(x) _GL_WARN_REAL_FLOATING_IMPL (isinf, x) # endif #endif #if @GNULIB_ISNANF@ /* Test for NaN for 'float' numbers. */ # if @HAVE_ISNANF@ /* The original included above provides a declaration of isnan macro or (older) isnanf function. */ # if __GNUC__ >= 4 /* GCC 4.0 and newer provides three built-ins for isnan. */ # undef isnanf # define isnanf(x) __builtin_isnanf ((float)(x)) # elif defined isnan # undef isnanf # define isnanf(x) isnan ((float)(x)) # endif # else /* Test whether X is a NaN. */ # undef isnanf # define isnanf rpl_isnanf _GL_EXTERN_C int isnanf (float x); # endif #endif #if @GNULIB_ISNAND@ /* Test for NaN for 'double' numbers. This function is a gnulib extension, unlike isnan() which applied only to 'double' numbers earlier but now is a type-generic macro. */ # if @HAVE_ISNAND@ /* The original included above provides a declaration of isnan macro. */ # if __GNUC__ >= 4 /* GCC 4.0 and newer provides three built-ins for isnan. */ # undef isnand # define isnand(x) __builtin_isnan ((double)(x)) # else # undef isnand # define isnand(x) isnan ((double)(x)) # endif # else /* Test whether X is a NaN. */ # undef isnand # define isnand rpl_isnand _GL_EXTERN_C int isnand (double x); # endif #endif #if @GNULIB_ISNANL@ /* Test for NaN for 'long double' numbers. */ # if @HAVE_ISNANL@ /* The original included above provides a declaration of isnan macro or (older) isnanl function. */ # if __GNUC__ >= 4 /* GCC 4.0 and newer provides three built-ins for isnan. */ # undef isnanl # define isnanl(x) __builtin_isnanl ((long double)(x)) # elif defined isnan # undef isnanl # define isnanl(x) isnan ((long double)(x)) # endif # else /* Test whether X is a NaN. */ # undef isnanl # define isnanl rpl_isnanl _GL_EXTERN_C int isnanl (long double x) _GL_ATTRIBUTE_CONST; # endif #endif /* This must come *after* the snippets for GNULIB_ISNANF and GNULIB_ISNANL! */ #if @GNULIB_ISNAN@ # if @REPLACE_ISNAN@ /* We can't just use the isnanf macro (e.g.) as exposed by isnanf.h (e.g.) here, because those may end up being macros that recursively expand back to isnan. So use the gnulib replacements for them directly. */ # if @HAVE_ISNANF@ && __GNUC__ >= 4 # define gl_isnan_f(x) __builtin_isnanf ((float)(x)) # else _GL_EXTERN_C int rpl_isnanf (float x); # define gl_isnan_f(x) rpl_isnanf (x) # endif # if @HAVE_ISNAND@ && __GNUC__ >= 4 # define gl_isnan_d(x) __builtin_isnan ((double)(x)) # else _GL_EXTERN_C int rpl_isnand (double x); # define gl_isnan_d(x) rpl_isnand (x) # endif # if @HAVE_ISNANL@ && __GNUC__ >= 4 # define gl_isnan_l(x) __builtin_isnanl ((long double)(x)) # else _GL_EXTERN_C int rpl_isnanl (long double x) _GL_ATTRIBUTE_CONST; # define gl_isnan_l(x) rpl_isnanl (x) # endif # undef isnan # define isnan(x) \ (sizeof (x) == sizeof (long double) ? gl_isnan_l (x) : \ sizeof (x) == sizeof (double) ? gl_isnan_d (x) : \ gl_isnan_f (x)) # elif __GNUC__ >= 4 # undef isnan # define isnan(x) \ (sizeof (x) == sizeof (long double) ? __builtin_isnanl ((long double)(x)) : \ sizeof (x) == sizeof (double) ? __builtin_isnan ((double)(x)) : \ __builtin_isnanf ((float)(x))) # endif # ifdef __cplusplus # ifdef isnan _GL_MATH_CXX_REAL_FLOATING_DECL_1 (isnan) # undef isnan _GL_MATH_CXX_REAL_FLOATING_DECL_2 (isnan) # endif # else /* Ensure isnan is a macro. */ # ifndef isnan # define isnan isnan # endif # endif #elif defined GNULIB_POSIXCHECK # if defined isnan _GL_WARN_REAL_FLOATING_DECL (isnan); # undef isnan # define isnan(x) _GL_WARN_REAL_FLOATING_IMPL (isnan, x) # endif #endif #if @GNULIB_SIGNBIT@ # if (@REPLACE_SIGNBIT_USING_GCC@ \ && (!defined __cplusplus || __cplusplus < 201103)) # undef signbit /* GCC 4.0 and newer provides three built-ins for signbit. */ # define signbit(x) \ (sizeof (x) == sizeof (long double) ? __builtin_signbitl (x) : \ sizeof (x) == sizeof (double) ? __builtin_signbit (x) : \ __builtin_signbitf (x)) # endif # if @REPLACE_SIGNBIT@ # undef signbit _GL_EXTERN_C int gl_signbitf (float arg); _GL_EXTERN_C int gl_signbitd (double arg); _GL_EXTERN_C int gl_signbitl (long double arg); # if __GNUC__ >= 2 && !defined __STRICT_ANSI__ # define _GL_NUM_UINT_WORDS(type) \ ((sizeof (type) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) # if defined FLT_SIGNBIT_WORD && defined FLT_SIGNBIT_BIT && !defined gl_signbitf # define gl_signbitf_OPTIMIZED_MACRO # define gl_signbitf(arg) \ ({ union { float _value; \ unsigned int _word[_GL_NUM_UINT_WORDS (float)]; \ } _m; \ _m._value = (arg); \ (_m._word[FLT_SIGNBIT_WORD] >> FLT_SIGNBIT_BIT) & 1; \ }) # endif # if defined DBL_SIGNBIT_WORD && defined DBL_SIGNBIT_BIT && !defined gl_signbitd # define gl_signbitd_OPTIMIZED_MACRO # define gl_signbitd(arg) \ ({ union { double _value; \ unsigned int _word[_GL_NUM_UINT_WORDS (double)]; \ } _m; \ _m._value = (arg); \ (_m._word[DBL_SIGNBIT_WORD] >> DBL_SIGNBIT_BIT) & 1; \ }) # endif # if defined LDBL_SIGNBIT_WORD && defined LDBL_SIGNBIT_BIT && !defined gl_signbitl # define gl_signbitl_OPTIMIZED_MACRO # define gl_signbitl(arg) \ ({ union { long double _value; \ unsigned int _word[_GL_NUM_UINT_WORDS (long double)]; \ } _m; \ _m._value = (arg); \ (_m._word[LDBL_SIGNBIT_WORD] >> LDBL_SIGNBIT_BIT) & 1; \ }) # endif # endif # define signbit(x) \ (sizeof (x) == sizeof (long double) ? gl_signbitl (x) : \ sizeof (x) == sizeof (double) ? gl_signbitd (x) : \ gl_signbitf (x)) # endif # ifdef __cplusplus # ifdef signbit _GL_MATH_CXX_REAL_FLOATING_DECL_1 (signbit) # undef signbit _GL_MATH_CXX_REAL_FLOATING_DECL_2 (signbit) # endif # endif #elif defined GNULIB_POSIXCHECK # if defined signbit _GL_WARN_REAL_FLOATING_DECL (signbit); # undef signbit # define signbit(x) _GL_WARN_REAL_FLOATING_IMPL (signbit, x) # endif #endif _GL_INLINE_HEADER_END #endif /* _@GUARD_PREFIX@_MATH_H */ #endif /* _@GUARD_PREFIX@_MATH_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/locale.in.h0000644000175000017500000001600213004436754016413 00000000000000/* A POSIX . Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #ifdef _GL_ALREADY_INCLUDING_LOCALE_H /* Special invocation conventions to handle Solaris header files (through Solaris 10) when combined with gettext's libintl.h. */ #@INCLUDE_NEXT@ @NEXT_LOCALE_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_LOCALE_H #define _GL_ALREADY_INCLUDING_LOCALE_H /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_LOCALE_H@ #undef _GL_ALREADY_INCLUDING_LOCALE_H #ifndef _@GUARD_PREFIX@_LOCALE_H #define _@GUARD_PREFIX@_LOCALE_H /* NetBSD 5.0 mis-defines NULL. */ #include /* Mac OS X 10.5 defines the locale_t type in . */ #if @HAVE_XLOCALE_H@ # include #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* The LC_MESSAGES locale category is specified in POSIX, but not in ISO C. On systems that don't define it, use the same value as GNU libintl. */ #if !defined LC_MESSAGES # define LC_MESSAGES 1729 #endif /* Bionic libc's 'struct lconv' is just a dummy. */ #if @REPLACE_STRUCT_LCONV@ # define lconv rpl_lconv struct lconv { /* All 'char *' are actually 'const char *'. */ /* Members that depend on the LC_NUMERIC category of the locale. See */ /* Symbol used as decimal point. */ char *decimal_point; /* Symbol used to separate groups of digits to the left of the decimal point. */ char *thousands_sep; /* Definition of the size of groups of digits to the left of the decimal point. */ char *grouping; /* Members that depend on the LC_MONETARY category of the locale. See */ /* Symbol used as decimal point. */ char *mon_decimal_point; /* Symbol used to separate groups of digits to the left of the decimal point. */ char *mon_thousands_sep; /* Definition of the size of groups of digits to the left of the decimal point. */ char *mon_grouping; /* Sign used to indicate a value >= 0. */ char *positive_sign; /* Sign used to indicate a value < 0. */ char *negative_sign; /* For formatting local currency. */ /* Currency symbol (3 characters) followed by separator (1 character). */ char *currency_symbol; /* Number of digits after the decimal point. */ char frac_digits; /* For values >= 0: 1 if the currency symbol precedes the number, 0 if it comes after the number. */ char p_cs_precedes; /* For values >= 0: Position of the sign. */ char p_sign_posn; /* For values >= 0: Placement of spaces between currency symbol, sign, and number. */ char p_sep_by_space; /* For values < 0: 1 if the currency symbol precedes the number, 0 if it comes after the number. */ char n_cs_precedes; /* For values < 0: Position of the sign. */ char n_sign_posn; /* For values < 0: Placement of spaces between currency symbol, sign, and number. */ char n_sep_by_space; /* For formatting international currency. */ /* Currency symbol (3 characters) followed by separator (1 character). */ char *int_curr_symbol; /* Number of digits after the decimal point. */ char int_frac_digits; /* For values >= 0: 1 if the currency symbol precedes the number, 0 if it comes after the number. */ char int_p_cs_precedes; /* For values >= 0: Position of the sign. */ char int_p_sign_posn; /* For values >= 0: Placement of spaces between currency symbol, sign, and number. */ char int_p_sep_by_space; /* For values < 0: 1 if the currency symbol precedes the number, 0 if it comes after the number. */ char int_n_cs_precedes; /* For values < 0: Position of the sign. */ char int_n_sign_posn; /* For values < 0: Placement of spaces between currency symbol, sign, and number. */ char int_n_sep_by_space; }; #endif #if @GNULIB_LOCALECONV@ # if @REPLACE_LOCALECONV@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef localeconv # define localeconv rpl_localeconv # endif _GL_FUNCDECL_RPL (localeconv, struct lconv *, (void)); _GL_CXXALIAS_RPL (localeconv, struct lconv *, (void)); # else _GL_CXXALIAS_SYS (localeconv, struct lconv *, (void)); # endif _GL_CXXALIASWARN (localeconv); #elif @REPLACE_STRUCT_LCONV@ # undef localeconv # define localeconv localeconv_used_without_requesting_gnulib_module_localeconv #elif defined GNULIB_POSIXCHECK # undef localeconv # if HAVE_RAW_DECL_LOCALECONV _GL_WARN_ON_USE (localeconv, "localeconv returns too few information on some platforms - " "use gnulib module localeconv for portability"); # endif #endif #if @GNULIB_SETLOCALE@ # if @REPLACE_SETLOCALE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef setlocale # define setlocale rpl_setlocale # define GNULIB_defined_setlocale 1 # endif _GL_FUNCDECL_RPL (setlocale, char *, (int category, const char *locale)); _GL_CXXALIAS_RPL (setlocale, char *, (int category, const char *locale)); # else _GL_CXXALIAS_SYS (setlocale, char *, (int category, const char *locale)); # endif _GL_CXXALIASWARN (setlocale); #elif defined GNULIB_POSIXCHECK # undef setlocale # if HAVE_RAW_DECL_SETLOCALE _GL_WARN_ON_USE (setlocale, "setlocale works differently on native Windows - " "use gnulib module setlocale for portability"); # endif #endif #if @GNULIB_DUPLOCALE@ # if @REPLACE_DUPLOCALE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef duplocale # define duplocale rpl_duplocale # endif _GL_FUNCDECL_RPL (duplocale, locale_t, (locale_t locale) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (duplocale, locale_t, (locale_t locale)); # else # if @HAVE_DUPLOCALE@ _GL_CXXALIAS_SYS (duplocale, locale_t, (locale_t locale)); # endif # endif # if @HAVE_DUPLOCALE@ _GL_CXXALIASWARN (duplocale); # endif #elif defined GNULIB_POSIXCHECK # undef duplocale # if HAVE_RAW_DECL_DUPLOCALE _GL_WARN_ON_USE (duplocale, "duplocale is buggy on some glibc systems - " "use gnulib module duplocale for portability"); # endif #endif #endif /* _@GUARD_PREFIX@_LOCALE_H */ #endif /* ! _GL_ALREADY_INCLUDING_LOCALE_H */ #endif /* _@GUARD_PREFIX@_LOCALE_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/ref-del.sin0000644000175000017500000000167513004436754016441 00000000000000# Remove this package from a list of references stored in a text file. # # Copyright (C) 2000, 2009-2016 Free Software Foundation, Inc. # # This program is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3, or (at your option) # any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License along # with this program; if not, see . # # Written by Bruno Haible . # /^# Packages using this file: / { s/# Packages using this file:// s/ @PACKAGE@ / / s/^/# Packages using this file:/ } gnuastro-0.2.33-8a3b/bootstrapped/lib/ref-add.sin0000644000175000017500000000175213004436754016421 00000000000000# Add this package to a list of references stored in a text file. # # Copyright (C) 2000, 2009-2016 Free Software Foundation, Inc. # # This program is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3, or (at your option) # any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License along # with this program; if not, see . # # Written by Bruno Haible . # /^# Packages using this file: / { s/# Packages using this file:// ta :a s/ @PACKAGE@ / @PACKAGE@ / tb s/ $/ @PACKAGE@ / :b s/^/# Packages using this file:/ } gnuastro-0.2.33-8a3b/bootstrapped/lib/config.charset0000644000175000017500000005473613004436754017236 00000000000000#! /bin/sh # Output a system dependent table of character encoding aliases. # # Copyright (C) 2000-2004, 2006-2016 Free Software Foundation, Inc. # # This program is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3, or (at your option) # any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License along # with this program; if not, see . # # The table consists of lines of the form # ALIAS CANONICAL # # ALIAS is the (system dependent) result of "nl_langinfo (CODESET)". # ALIAS is compared in a case sensitive way. # # CANONICAL is the GNU canonical name for this character encoding. # It must be an encoding supported by libiconv. Support by GNU libc is # also desirable. CANONICAL is case insensitive. Usually an upper case # MIME charset name is preferred. # The current list of GNU canonical charset names is as follows. # # name MIME? used by which systems # (darwin = Mac OS X, woe32 = native Windows) # # ASCII, ANSI_X3.4-1968 glibc solaris freebsd netbsd darwin cygwin # ISO-8859-1 Y glibc aix hpux irix osf solaris freebsd netbsd openbsd darwin cygwin # ISO-8859-2 Y glibc aix hpux irix osf solaris freebsd netbsd openbsd darwin cygwin # ISO-8859-3 Y glibc solaris cygwin # ISO-8859-4 Y osf solaris freebsd netbsd openbsd darwin # ISO-8859-5 Y glibc aix hpux irix osf solaris freebsd netbsd openbsd darwin cygwin # ISO-8859-6 Y glibc aix hpux solaris cygwin # ISO-8859-7 Y glibc aix hpux irix osf solaris netbsd openbsd darwin cygwin # ISO-8859-8 Y glibc aix hpux osf solaris cygwin # ISO-8859-9 Y glibc aix hpux irix osf solaris darwin cygwin # ISO-8859-13 glibc netbsd openbsd darwin cygwin # ISO-8859-14 glibc cygwin # ISO-8859-15 glibc aix osf solaris freebsd netbsd openbsd darwin cygwin # KOI8-R Y glibc solaris freebsd netbsd openbsd darwin # KOI8-U Y glibc freebsd netbsd openbsd darwin cygwin # KOI8-T glibc # CP437 dos # CP775 dos # CP850 aix osf dos # CP852 dos # CP855 dos # CP856 aix # CP857 dos # CP861 dos # CP862 dos # CP864 dos # CP865 dos # CP866 freebsd netbsd openbsd darwin dos # CP869 dos # CP874 woe32 dos # CP922 aix # CP932 aix cygwin woe32 dos # CP943 aix # CP949 osf darwin woe32 dos # CP950 woe32 dos # CP1046 aix # CP1124 aix # CP1125 dos # CP1129 aix # CP1131 darwin # CP1250 woe32 # CP1251 glibc solaris netbsd openbsd darwin cygwin woe32 # CP1252 aix woe32 # CP1253 woe32 # CP1254 woe32 # CP1255 glibc woe32 # CP1256 woe32 # CP1257 woe32 # GB2312 Y glibc aix hpux irix solaris freebsd netbsd darwin # EUC-JP Y glibc aix hpux irix osf solaris freebsd netbsd darwin # EUC-KR Y glibc aix hpux irix osf solaris freebsd netbsd darwin cygwin # EUC-TW glibc aix hpux irix osf solaris netbsd # BIG5 Y glibc aix hpux osf solaris freebsd netbsd darwin cygwin # BIG5-HKSCS glibc solaris darwin # GBK glibc aix osf solaris darwin cygwin woe32 dos # GB18030 glibc solaris netbsd darwin # SHIFT_JIS Y hpux osf solaris freebsd netbsd darwin # JOHAB glibc solaris woe32 # TIS-620 glibc aix hpux osf solaris cygwin # VISCII Y glibc # TCVN5712-1 glibc # ARMSCII-8 glibc darwin # GEORGIAN-PS glibc cygwin # PT154 glibc # HP-ROMAN8 hpux # HP-ARABIC8 hpux # HP-GREEK8 hpux # HP-HEBREW8 hpux # HP-TURKISH8 hpux # HP-KANA8 hpux # DEC-KANJI osf # DEC-HANYU osf # UTF-8 Y glibc aix hpux osf solaris netbsd darwin cygwin # # Note: Names which are not marked as being a MIME name should not be used in # Internet protocols for information interchange (mail, news, etc.). # # Note: ASCII and ANSI_X3.4-1968 are synonymous canonical names. Applications # must understand both names and treat them as equivalent. # # The first argument passed to this file is the canonical host specification, # CPU_TYPE-MANUFACTURER-OPERATING_SYSTEM # or # CPU_TYPE-MANUFACTURER-KERNEL-OPERATING_SYSTEM host="$1" os=`echo "$host" | sed -e 's/^[^-]*-[^-]*-\(.*\)$/\1/'` echo "# This file contains a table of character encoding aliases," echo "# suitable for operating system '${os}'." echo "# It was automatically generated from config.charset." # List of references, updated during installation: echo "# Packages using this file: " case "$os" in linux-gnulibc1*) # Linux libc5 doesn't have nl_langinfo(CODESET); therefore # localcharset.c falls back to using the full locale name # from the environment variables. echo "C ASCII" echo "POSIX ASCII" for l in af af_ZA ca ca_ES da da_DK de de_AT de_BE de_CH de_DE de_LU \ en en_AU en_BW en_CA en_DK en_GB en_IE en_NZ en_US en_ZA \ en_ZW es es_AR es_BO es_CL es_CO es_DO es_EC es_ES es_GT \ es_HN es_MX es_PA es_PE es_PY es_SV es_US es_UY es_VE et \ et_EE eu eu_ES fi fi_FI fo fo_FO fr fr_BE fr_CA fr_CH fr_FR \ fr_LU ga ga_IE gl gl_ES id id_ID in in_ID is is_IS it it_CH \ it_IT kl kl_GL nl nl_BE nl_NL no no_NO pt pt_BR pt_PT sv \ sv_FI sv_SE; do echo "$l ISO-8859-1" echo "$l.iso-8859-1 ISO-8859-1" echo "$l.iso-8859-15 ISO-8859-15" echo "$l.iso-8859-15@euro ISO-8859-15" echo "$l@euro ISO-8859-15" echo "$l.cp-437 CP437" echo "$l.cp-850 CP850" echo "$l.cp-1252 CP1252" echo "$l.cp-1252@euro CP1252" #echo "$l.atari-st ATARI-ST" # not a commonly used encoding echo "$l.utf-8 UTF-8" echo "$l.utf-8@euro UTF-8" done for l in cs cs_CZ hr hr_HR hu hu_HU pl pl_PL ro ro_RO sk sk_SK sl \ sl_SI sr sr_CS sr_YU; do echo "$l ISO-8859-2" echo "$l.iso-8859-2 ISO-8859-2" echo "$l.cp-852 CP852" echo "$l.cp-1250 CP1250" echo "$l.utf-8 UTF-8" done for l in mk mk_MK ru ru_RU; do echo "$l ISO-8859-5" echo "$l.iso-8859-5 ISO-8859-5" echo "$l.koi8-r KOI8-R" echo "$l.cp-866 CP866" echo "$l.cp-1251 CP1251" echo "$l.utf-8 UTF-8" done for l in ar ar_SA; do echo "$l ISO-8859-6" echo "$l.iso-8859-6 ISO-8859-6" echo "$l.cp-864 CP864" #echo "$l.cp-868 CP868" # not a commonly used encoding echo "$l.cp-1256 CP1256" echo "$l.utf-8 UTF-8" done for l in el el_GR gr gr_GR; do echo "$l ISO-8859-7" echo "$l.iso-8859-7 ISO-8859-7" echo "$l.cp-869 CP869" echo "$l.cp-1253 CP1253" echo "$l.cp-1253@euro CP1253" echo "$l.utf-8 UTF-8" echo "$l.utf-8@euro UTF-8" done for l in he he_IL iw iw_IL; do echo "$l ISO-8859-8" echo "$l.iso-8859-8 ISO-8859-8" echo "$l.cp-862 CP862" echo "$l.cp-1255 CP1255" echo "$l.utf-8 UTF-8" done for l in tr tr_TR; do echo "$l ISO-8859-9" echo "$l.iso-8859-9 ISO-8859-9" echo "$l.cp-857 CP857" echo "$l.cp-1254 CP1254" echo "$l.utf-8 UTF-8" done for l in lt lt_LT lv lv_LV; do #echo "$l BALTIC" # not a commonly used encoding, wrong encoding name echo "$l ISO-8859-13" done for l in ru_UA uk uk_UA; do echo "$l KOI8-U" done for l in zh zh_CN; do #echo "$l GB_2312-80" # not a commonly used encoding, wrong encoding name echo "$l GB2312" done for l in ja ja_JP ja_JP.EUC; do echo "$l EUC-JP" done for l in ko ko_KR; do echo "$l EUC-KR" done for l in th th_TH; do echo "$l TIS-620" done for l in fa fa_IR; do #echo "$l ISIRI-3342" # a broken encoding echo "$l.utf-8 UTF-8" done ;; linux* | *-gnu*) # With glibc-2.1 or newer, we don't need any canonicalization, # because glibc has iconv and both glibc and libiconv support all # GNU canonical names directly. Therefore, the Makefile does not # need to install the alias file at all. # The following applies only to glibc-2.0.x and older libcs. echo "ISO_646.IRV:1983 ASCII" ;; aix*) echo "ISO8859-1 ISO-8859-1" echo "ISO8859-2 ISO-8859-2" echo "ISO8859-5 ISO-8859-5" echo "ISO8859-6 ISO-8859-6" echo "ISO8859-7 ISO-8859-7" echo "ISO8859-8 ISO-8859-8" echo "ISO8859-9 ISO-8859-9" echo "ISO8859-15 ISO-8859-15" echo "IBM-850 CP850" echo "IBM-856 CP856" echo "IBM-921 ISO-8859-13" echo "IBM-922 CP922" echo "IBM-932 CP932" echo "IBM-943 CP943" echo "IBM-1046 CP1046" echo "IBM-1124 CP1124" echo "IBM-1129 CP1129" echo "IBM-1252 CP1252" echo "IBM-eucCN GB2312" echo "IBM-eucJP EUC-JP" echo "IBM-eucKR EUC-KR" echo "IBM-eucTW EUC-TW" echo "big5 BIG5" echo "GBK GBK" echo "TIS-620 TIS-620" echo "UTF-8 UTF-8" ;; hpux*) echo "iso88591 ISO-8859-1" echo "iso88592 ISO-8859-2" echo "iso88595 ISO-8859-5" echo "iso88596 ISO-8859-6" echo "iso88597 ISO-8859-7" echo "iso88598 ISO-8859-8" echo "iso88599 ISO-8859-9" echo "iso885915 ISO-8859-15" echo "roman8 HP-ROMAN8" echo "arabic8 HP-ARABIC8" echo "greek8 HP-GREEK8" echo "hebrew8 HP-HEBREW8" echo "turkish8 HP-TURKISH8" echo "kana8 HP-KANA8" echo "tis620 TIS-620" echo "big5 BIG5" echo "eucJP EUC-JP" echo "eucKR EUC-KR" echo "eucTW EUC-TW" echo "hp15CN GB2312" #echo "ccdc ?" # what is this? echo "SJIS SHIFT_JIS" echo "utf8 UTF-8" ;; irix*) echo "ISO8859-1 ISO-8859-1" echo "ISO8859-2 ISO-8859-2" echo "ISO8859-5 ISO-8859-5" echo "ISO8859-7 ISO-8859-7" echo "ISO8859-9 ISO-8859-9" echo "eucCN GB2312" echo "eucJP EUC-JP" echo "eucKR EUC-KR" echo "eucTW EUC-TW" ;; osf*) echo "ISO8859-1 ISO-8859-1" echo "ISO8859-2 ISO-8859-2" echo "ISO8859-4 ISO-8859-4" echo "ISO8859-5 ISO-8859-5" echo "ISO8859-7 ISO-8859-7" echo "ISO8859-8 ISO-8859-8" echo "ISO8859-9 ISO-8859-9" echo "ISO8859-15 ISO-8859-15" echo "cp850 CP850" echo "big5 BIG5" echo "dechanyu DEC-HANYU" echo "dechanzi GB2312" echo "deckanji DEC-KANJI" echo "deckorean EUC-KR" echo "eucJP EUC-JP" echo "eucKR EUC-KR" echo "eucTW EUC-TW" echo "GBK GBK" echo "KSC5601 CP949" echo "sdeckanji EUC-JP" echo "SJIS SHIFT_JIS" echo "TACTIS TIS-620" echo "UTF-8 UTF-8" ;; solaris*) echo "646 ASCII" echo "ISO8859-1 ISO-8859-1" echo "ISO8859-2 ISO-8859-2" echo "ISO8859-3 ISO-8859-3" echo "ISO8859-4 ISO-8859-4" echo "ISO8859-5 ISO-8859-5" echo "ISO8859-6 ISO-8859-6" echo "ISO8859-7 ISO-8859-7" echo "ISO8859-8 ISO-8859-8" echo "ISO8859-9 ISO-8859-9" echo "ISO8859-15 ISO-8859-15" echo "koi8-r KOI8-R" echo "ansi-1251 CP1251" echo "BIG5 BIG5" echo "Big5-HKSCS BIG5-HKSCS" echo "gb2312 GB2312" echo "GBK GBK" echo "GB18030 GB18030" echo "cns11643 EUC-TW" echo "5601 EUC-KR" echo "ko_KR.johap92 JOHAB" echo "eucJP EUC-JP" echo "PCK SHIFT_JIS" echo "TIS620.2533 TIS-620" #echo "sun_eu_greek ?" # what is this? echo "UTF-8 UTF-8" ;; freebsd*) # FreeBSD 4.2 doesn't have nl_langinfo(CODESET); therefore # localcharset.c falls back to using the full locale name # from the environment variables. echo "C ASCII" echo "US-ASCII ASCII" for l in la_LN lt_LN; do echo "$l.ASCII ASCII" done for l in da_DK de_AT de_CH de_DE en_AU en_CA en_GB en_US es_ES \ fi_FI fr_BE fr_CA fr_CH fr_FR is_IS it_CH it_IT la_LN \ lt_LN nl_BE nl_NL no_NO pt_PT sv_SE; do echo "$l.ISO_8859-1 ISO-8859-1" echo "$l.DIS_8859-15 ISO-8859-15" done for l in cs_CZ hr_HR hu_HU la_LN lt_LN pl_PL sl_SI; do echo "$l.ISO_8859-2 ISO-8859-2" done for l in la_LN lt_LT; do echo "$l.ISO_8859-4 ISO-8859-4" done for l in ru_RU ru_SU; do echo "$l.KOI8-R KOI8-R" echo "$l.ISO_8859-5 ISO-8859-5" echo "$l.CP866 CP866" done echo "uk_UA.KOI8-U KOI8-U" echo "zh_TW.BIG5 BIG5" echo "zh_TW.Big5 BIG5" echo "zh_CN.EUC GB2312" echo "ja_JP.EUC EUC-JP" echo "ja_JP.SJIS SHIFT_JIS" echo "ja_JP.Shift_JIS SHIFT_JIS" echo "ko_KR.EUC EUC-KR" ;; netbsd*) echo "646 ASCII" echo "ISO8859-1 ISO-8859-1" echo "ISO8859-2 ISO-8859-2" echo "ISO8859-4 ISO-8859-4" echo "ISO8859-5 ISO-8859-5" echo "ISO8859-7 ISO-8859-7" echo "ISO8859-13 ISO-8859-13" echo "ISO8859-15 ISO-8859-15" echo "eucCN GB2312" echo "eucJP EUC-JP" echo "eucKR EUC-KR" echo "eucTW EUC-TW" echo "BIG5 BIG5" echo "SJIS SHIFT_JIS" ;; openbsd*) echo "646 ASCII" echo "ISO8859-1 ISO-8859-1" echo "ISO8859-2 ISO-8859-2" echo "ISO8859-4 ISO-8859-4" echo "ISO8859-5 ISO-8859-5" echo "ISO8859-7 ISO-8859-7" echo "ISO8859-13 ISO-8859-13" echo "ISO8859-15 ISO-8859-15" ;; darwin[56]*) # Darwin 6.8 doesn't have nl_langinfo(CODESET); therefore # localcharset.c falls back to using the full locale name # from the environment variables. echo "C ASCII" for l in en_AU en_CA en_GB en_US la_LN; do echo "$l.US-ASCII ASCII" done for l in da_DK de_AT de_CH de_DE en_AU en_CA en_GB en_US es_ES \ fi_FI fr_BE fr_CA fr_CH fr_FR is_IS it_CH it_IT nl_BE \ nl_NL no_NO pt_PT sv_SE; do echo "$l ISO-8859-1" echo "$l.ISO8859-1 ISO-8859-1" echo "$l.ISO8859-15 ISO-8859-15" done for l in la_LN; do echo "$l.ISO8859-1 ISO-8859-1" echo "$l.ISO8859-15 ISO-8859-15" done for l in cs_CZ hr_HR hu_HU la_LN pl_PL sl_SI; do echo "$l.ISO8859-2 ISO-8859-2" done for l in la_LN lt_LT; do echo "$l.ISO8859-4 ISO-8859-4" done for l in ru_RU; do echo "$l.KOI8-R KOI8-R" echo "$l.ISO8859-5 ISO-8859-5" echo "$l.CP866 CP866" done for l in bg_BG; do echo "$l.CP1251 CP1251" done echo "uk_UA.KOI8-U KOI8-U" echo "zh_TW.BIG5 BIG5" echo "zh_TW.Big5 BIG5" echo "zh_CN.EUC GB2312" echo "ja_JP.EUC EUC-JP" echo "ja_JP.SJIS SHIFT_JIS" echo "ko_KR.EUC EUC-KR" ;; darwin*) # Darwin 7.5 has nl_langinfo(CODESET), but sometimes its value is # useless: # - It returns the empty string when LANG is set to a locale of the # form ll_CC, although ll_CC/LC_CTYPE is a symlink to an UTF-8 # LC_CTYPE file. # - The environment variables LANG, LC_CTYPE, LC_ALL are not set by # the system; nl_langinfo(CODESET) returns "US-ASCII" in this case. # - The documentation says: # "... all code that calls BSD system routines should ensure # that the const *char parameters of these routines are in UTF-8 # encoding. All BSD system functions expect their string # parameters to be in UTF-8 encoding and nothing else." # It also says # "An additional caveat is that string parameters for files, # paths, and other file-system entities must be in canonical # UTF-8. In a canonical UTF-8 Unicode string, all decomposable # characters are decomposed ..." # but this is not true: You can pass non-decomposed UTF-8 strings # to file system functions, and it is the OS which will convert # them to decomposed UTF-8 before accessing the file system. # - The Apple Terminal application displays UTF-8 by default. # - However, other applications are free to use different encodings: # - xterm uses ISO-8859-1 by default. # - TextEdit uses MacRoman by default. # We prefer UTF-8 over decomposed UTF-8-MAC because one should # minimize the use of decomposed Unicode. Unfortunately, through the # Darwin file system, decomposed UTF-8 strings are leaked into user # space nevertheless. # Then there are also the locales with encodings other than US-ASCII # and UTF-8. These locales can be occasionally useful to users (e.g. # when grepping through ISO-8859-1 encoded text files), when all their # file names are in US-ASCII. echo "ISO8859-1 ISO-8859-1" echo "ISO8859-2 ISO-8859-2" echo "ISO8859-4 ISO-8859-4" echo "ISO8859-5 ISO-8859-5" echo "ISO8859-7 ISO-8859-7" echo "ISO8859-9 ISO-8859-9" echo "ISO8859-13 ISO-8859-13" echo "ISO8859-15 ISO-8859-15" echo "KOI8-R KOI8-R" echo "KOI8-U KOI8-U" echo "CP866 CP866" echo "CP949 CP949" echo "CP1131 CP1131" echo "CP1251 CP1251" echo "eucCN GB2312" echo "GB2312 GB2312" echo "eucJP EUC-JP" echo "eucKR EUC-KR" echo "Big5 BIG5" echo "Big5HKSCS BIG5-HKSCS" echo "GBK GBK" echo "GB18030 GB18030" echo "SJIS SHIFT_JIS" echo "ARMSCII-8 ARMSCII-8" echo "PT154 PT154" #echo "ISCII-DEV ?" echo "* UTF-8" ;; beos* | haiku*) # BeOS and Haiku have a single locale, and it has UTF-8 encoding. echo "* UTF-8" ;; msdosdjgpp*) # DJGPP 2.03 doesn't have nl_langinfo(CODESET); therefore # localcharset.c falls back to using the full locale name # from the environment variables. echo "#" echo "# The encodings given here may not all be correct." echo "# If you find that the encoding given for your language and" echo "# country is not the one your DOS machine actually uses, just" echo "# correct it in this file, and send a mail to" echo "# Juan Manuel Guerrero " echo "# and Bruno Haible ." echo "#" echo "C ASCII" # ISO-8859-1 languages echo "ca CP850" echo "ca_ES CP850" echo "da CP865" # not CP850 ?? echo "da_DK CP865" # not CP850 ?? echo "de CP850" echo "de_AT CP850" echo "de_CH CP850" echo "de_DE CP850" echo "en CP850" echo "en_AU CP850" # not CP437 ?? echo "en_CA CP850" echo "en_GB CP850" echo "en_NZ CP437" echo "en_US CP437" echo "en_ZA CP850" # not CP437 ?? echo "es CP850" echo "es_AR CP850" echo "es_BO CP850" echo "es_CL CP850" echo "es_CO CP850" echo "es_CR CP850" echo "es_CU CP850" echo "es_DO CP850" echo "es_EC CP850" echo "es_ES CP850" echo "es_GT CP850" echo "es_HN CP850" echo "es_MX CP850" echo "es_NI CP850" echo "es_PA CP850" echo "es_PY CP850" echo "es_PE CP850" echo "es_SV CP850" echo "es_UY CP850" echo "es_VE CP850" echo "et CP850" echo "et_EE CP850" echo "eu CP850" echo "eu_ES CP850" echo "fi CP850" echo "fi_FI CP850" echo "fr CP850" echo "fr_BE CP850" echo "fr_CA CP850" echo "fr_CH CP850" echo "fr_FR CP850" echo "ga CP850" echo "ga_IE CP850" echo "gd CP850" echo "gd_GB CP850" echo "gl CP850" echo "gl_ES CP850" echo "id CP850" # not CP437 ?? echo "id_ID CP850" # not CP437 ?? echo "is CP861" # not CP850 ?? echo "is_IS CP861" # not CP850 ?? echo "it CP850" echo "it_CH CP850" echo "it_IT CP850" echo "lt CP775" echo "lt_LT CP775" echo "lv CP775" echo "lv_LV CP775" echo "nb CP865" # not CP850 ?? echo "nb_NO CP865" # not CP850 ?? echo "nl CP850" echo "nl_BE CP850" echo "nl_NL CP850" echo "nn CP865" # not CP850 ?? echo "nn_NO CP865" # not CP850 ?? echo "no CP865" # not CP850 ?? echo "no_NO CP865" # not CP850 ?? echo "pt CP850" echo "pt_BR CP850" echo "pt_PT CP850" echo "sv CP850" echo "sv_SE CP850" # ISO-8859-2 languages echo "cs CP852" echo "cs_CZ CP852" echo "hr CP852" echo "hr_HR CP852" echo "hu CP852" echo "hu_HU CP852" echo "pl CP852" echo "pl_PL CP852" echo "ro CP852" echo "ro_RO CP852" echo "sk CP852" echo "sk_SK CP852" echo "sl CP852" echo "sl_SI CP852" echo "sq CP852" echo "sq_AL CP852" echo "sr CP852" # CP852 or CP866 or CP855 ?? echo "sr_CS CP852" # CP852 or CP866 or CP855 ?? echo "sr_YU CP852" # CP852 or CP866 or CP855 ?? # ISO-8859-3 languages echo "mt CP850" echo "mt_MT CP850" # ISO-8859-5 languages echo "be CP866" echo "be_BE CP866" echo "bg CP866" # not CP855 ?? echo "bg_BG CP866" # not CP855 ?? echo "mk CP866" # not CP855 ?? echo "mk_MK CP866" # not CP855 ?? echo "ru CP866" echo "ru_RU CP866" echo "uk CP1125" echo "uk_UA CP1125" # ISO-8859-6 languages echo "ar CP864" echo "ar_AE CP864" echo "ar_DZ CP864" echo "ar_EG CP864" echo "ar_IQ CP864" echo "ar_IR CP864" echo "ar_JO CP864" echo "ar_KW CP864" echo "ar_MA CP864" echo "ar_OM CP864" echo "ar_QA CP864" echo "ar_SA CP864" echo "ar_SY CP864" # ISO-8859-7 languages echo "el CP869" echo "el_GR CP869" # ISO-8859-8 languages echo "he CP862" echo "he_IL CP862" # ISO-8859-9 languages echo "tr CP857" echo "tr_TR CP857" # Japanese echo "ja CP932" echo "ja_JP CP932" # Chinese echo "zh_CN GBK" echo "zh_TW CP950" # not CP938 ?? # Korean echo "kr CP949" # not CP934 ?? echo "kr_KR CP949" # not CP934 ?? # Thai echo "th CP874" echo "th_TH CP874" # Other echo "eo CP850" echo "eo_EO CP850" ;; esac gnuastro-0.2.33-8a3b/bootstrapped/lib/limits.in.h0000644000175000017500000000537613004436754016471 00000000000000/* A GNU-like . Copyright 2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _@GUARD_PREFIX@_LIMITS_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_LIMITS_H@ #ifndef _@GUARD_PREFIX@_LIMITS_H #define _@GUARD_PREFIX@_LIMITS_H /* The number of usable bits in an unsigned or signed integer type with minimum value MIN and maximum value MAX, as an int expression suitable in #if. Cover all known practical hosts. This implementation exploits the fact that MAX is 1 less than a power of 2, and merely counts the number of 1 bits in MAX; "COBn" means "count the number of 1 bits in the low-order n bits"). */ #define _GL_INTEGER_WIDTH(min, max) (((min) < 0) + _GL_COB128 (max)) #define _GL_COB128(n) (_GL_COB64 ((n) >> 31 >> 31 >> 2) + _GL_COB64 (n)) #define _GL_COB64(n) (_GL_COB32 ((n) >> 31 >> 1) + _GL_COB32 (n)) #define _GL_COB32(n) (_GL_COB16 ((n) >> 16) + _GL_COB16 (n)) #define _GL_COB16(n) (_GL_COB8 ((n) >> 8) + _GL_COB8 (n)) #define _GL_COB8(n) (_GL_COB4 ((n) >> 4) + _GL_COB4 (n)) #define _GL_COB4(n) (!!((n) & 8) + !!((n) & 4) + !!((n) & 2) + !!((n) & 1)) /* Macros specified by ISO/IEC TS 18661-1:2014. */ #if (! defined ULLONG_WIDTH \ && (defined _GNU_SOURCE || defined __STDC_WANT_IEC_60559_BFP_EXT__)) # define CHAR_WIDTH _GL_INTEGER_WIDTH (CHAR_MIN, CHAR_MAX) # define SCHAR_WIDTH _GL_INTEGER_WIDTH (SCHAR_MIN, SCHAR_MAX) # define UCHAR_WIDTH _GL_INTEGER_WIDTH (0, UCHAR_MAX) # define SHRT_WIDTH _GL_INTEGER_WIDTH (SHRT_MIN, SHRT_MAX) # define USHRT_WIDTH _GL_INTEGER_WIDTH (0, USHRT_MAX) # define INT_WIDTH _GL_INTEGER_WIDTH (INT_MIN, INT_MAX) # define UINT_WIDTH _GL_INTEGER_WIDTH (0, UINT_MAX) # define LONG_WIDTH _GL_INTEGER_WIDTH (LONG_MIN, LONG_MAX) # define ULONG_WIDTH _GL_INTEGER_WIDTH (0, ULONG_MAX) # define LLONG_WIDTH _GL_INTEGER_WIDTH (LLONG_MIN, LLONG_MAX) # define ULLONG_WIDTH _GL_INTEGER_WIDTH (0, ULLONG_MAX) #endif /* !ULLONG_WIDTH && (_GNU_SOURCE || __STDC_WANT_IEC_60559_BFP_EXT__) */ #endif /* _@GUARD_PREFIX@_LIMITS_H */ #endif /* _@GUARD_PREFIX@_LIMITS_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/langinfo.in.h0000644000175000017500000001321213004436754016751 00000000000000/* Substitute for and wrapper around . Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* * POSIX for platforms that lack it or have an incomplete one. * */ #ifndef _@GUARD_PREFIX@_LANGINFO_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* The include_next requires a split double-inclusion guard. */ #if @HAVE_LANGINFO_H@ # @INCLUDE_NEXT@ @NEXT_LANGINFO_H@ #endif #ifndef _@GUARD_PREFIX@_LANGINFO_H #define _@GUARD_PREFIX@_LANGINFO_H #if !@HAVE_LANGINFO_H@ /* A platform that lacks . */ /* Assume that it also lacks and the nl_item type. */ # if !GNULIB_defined_nl_item typedef int nl_item; # define GNULIB_defined_nl_item 1 # endif /* nl_langinfo items of the LC_CTYPE category */ # define CODESET 10000 /* nl_langinfo items of the LC_NUMERIC category */ # define RADIXCHAR 10001 # define DECIMAL_POINT RADIXCHAR # define THOUSEP 10002 # define THOUSANDS_SEP THOUSEP # define GROUPING 10114 /* nl_langinfo items of the LC_TIME category */ # define D_T_FMT 10003 # define D_FMT 10004 # define T_FMT 10005 # define T_FMT_AMPM 10006 # define AM_STR 10007 # define PM_STR 10008 # define DAY_1 10009 # define DAY_2 (DAY_1 + 1) # define DAY_3 (DAY_1 + 2) # define DAY_4 (DAY_1 + 3) # define DAY_5 (DAY_1 + 4) # define DAY_6 (DAY_1 + 5) # define DAY_7 (DAY_1 + 6) # define ABDAY_1 10016 # define ABDAY_2 (ABDAY_1 + 1) # define ABDAY_3 (ABDAY_1 + 2) # define ABDAY_4 (ABDAY_1 + 3) # define ABDAY_5 (ABDAY_1 + 4) # define ABDAY_6 (ABDAY_1 + 5) # define ABDAY_7 (ABDAY_1 + 6) # define MON_1 10023 # define MON_2 (MON_1 + 1) # define MON_3 (MON_1 + 2) # define MON_4 (MON_1 + 3) # define MON_5 (MON_1 + 4) # define MON_6 (MON_1 + 5) # define MON_7 (MON_1 + 6) # define MON_8 (MON_1 + 7) # define MON_9 (MON_1 + 8) # define MON_10 (MON_1 + 9) # define MON_11 (MON_1 + 10) # define MON_12 (MON_1 + 11) # define ABMON_1 10035 # define ABMON_2 (ABMON_1 + 1) # define ABMON_3 (ABMON_1 + 2) # define ABMON_4 (ABMON_1 + 3) # define ABMON_5 (ABMON_1 + 4) # define ABMON_6 (ABMON_1 + 5) # define ABMON_7 (ABMON_1 + 6) # define ABMON_8 (ABMON_1 + 7) # define ABMON_9 (ABMON_1 + 8) # define ABMON_10 (ABMON_1 + 9) # define ABMON_11 (ABMON_1 + 10) # define ABMON_12 (ABMON_1 + 11) # define ERA 10047 # define ERA_D_FMT 10048 # define ERA_D_T_FMT 10049 # define ERA_T_FMT 10050 # define ALT_DIGITS 10051 /* nl_langinfo items of the LC_MONETARY category */ # define CRNCYSTR 10052 # define CURRENCY_SYMBOL CRNCYSTR # define INT_CURR_SYMBOL 10100 # define MON_DECIMAL_POINT 10101 # define MON_THOUSANDS_SEP 10102 # define MON_GROUPING 10103 # define POSITIVE_SIGN 10104 # define NEGATIVE_SIGN 10105 # define FRAC_DIGITS 10106 # define INT_FRAC_DIGITS 10107 # define P_CS_PRECEDES 10108 # define N_CS_PRECEDES 10109 # define P_SEP_BY_SPACE 10110 # define N_SEP_BY_SPACE 10111 # define P_SIGN_POSN 10112 # define N_SIGN_POSN 10113 /* nl_langinfo items of the LC_MESSAGES category */ # define YESEXPR 10053 # define NOEXPR 10054 #else /* A platform that has . */ # if !@HAVE_LANGINFO_CODESET@ # define CODESET 10000 # define GNULIB_defined_CODESET 1 # endif # if !@HAVE_LANGINFO_T_FMT_AMPM@ # define T_FMT_AMPM 10006 # define GNULIB_defined_T_FMT_AMPM 1 # endif # if !@HAVE_LANGINFO_ERA@ # define ERA 10047 # define ERA_D_FMT 10048 # define ERA_D_T_FMT 10049 # define ERA_T_FMT 10050 # define ALT_DIGITS 10051 # define GNULIB_defined_ERA 1 # endif # if !@HAVE_LANGINFO_YESEXPR@ # define YESEXPR 10053 # define NOEXPR 10054 # define GNULIB_defined_YESEXPR 1 # endif #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Declare overridden functions. */ /* Return a piece of locale dependent information. Note: The difference between nl_langinfo (CODESET) and locale_charset () is that the latter normalizes the encoding names to GNU conventions. */ #if @GNULIB_NL_LANGINFO@ # if @REPLACE_NL_LANGINFO@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef nl_langinfo # define nl_langinfo rpl_nl_langinfo # endif _GL_FUNCDECL_RPL (nl_langinfo, char *, (nl_item item)); _GL_CXXALIAS_RPL (nl_langinfo, char *, (nl_item item)); # else # if !@HAVE_NL_LANGINFO@ _GL_FUNCDECL_SYS (nl_langinfo, char *, (nl_item item)); # endif _GL_CXXALIAS_SYS (nl_langinfo, char *, (nl_item item)); # endif _GL_CXXALIASWARN (nl_langinfo); #elif defined GNULIB_POSIXCHECK # undef nl_langinfo # if HAVE_RAW_DECL_NL_LANGINFO _GL_WARN_ON_USE (nl_langinfo, "nl_langinfo is not portable - " "use gnulib module nl_langinfo for portability"); # endif #endif #endif /* _@GUARD_PREFIX@_LANGINFO_H */ #endif /* _@GUARD_PREFIX@_LANGINFO_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/intprops.h0000644000175000017500000005124613004436754016436 00000000000000/* intprops.h -- properties of integer types Copyright (C) 2001-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paul Eggert. */ #ifndef _GL_INTPROPS_H #define _GL_INTPROPS_H #include #include #ifndef __has_builtin # define __has_builtin(x) 0 #endif /* Return a value with the common real type of E and V and the value of V. */ #define _GL_INT_CONVERT(e, v) (0 * (e) + (v)) /* Act like _GL_INT_CONVERT (E, -V) but work around a bug in IRIX 6.5 cc; see . */ #define _GL_INT_NEGATE_CONVERT(e, v) (0 * (e) - (v)) /* The extra casts in the following macros work around compiler bugs, e.g., in Cray C 5.0.3.0. */ /* True if the arithmetic type T is an integer type. bool counts as an integer. */ #define TYPE_IS_INTEGER(t) ((t) 1.5 == 1) /* True if the real type T is signed. */ #define TYPE_SIGNED(t) (! ((t) 0 < (t) -1)) /* Return 1 if the real expression E, after promotion, has a signed or floating type. */ #define EXPR_SIGNED(e) (_GL_INT_NEGATE_CONVERT (e, 1) < 0) /* Minimum and maximum values for integer types and expressions. */ /* The width in bits of the integer type or expression T. Padding bits are not supported; this is checked at compile-time below. */ #define TYPE_WIDTH(t) (sizeof (t) * CHAR_BIT) /* The maximum and minimum values for the integer type T. */ #define TYPE_MINIMUM(t) ((t) ~ TYPE_MAXIMUM (t)) #define TYPE_MAXIMUM(t) \ ((t) (! TYPE_SIGNED (t) \ ? (t) -1 \ : ((((t) 1 << (TYPE_WIDTH (t) - 2)) - 1) * 2 + 1))) /* The maximum and minimum values for the type of the expression E, after integer promotion. E should not have side effects. */ #define _GL_INT_MINIMUM(e) \ (EXPR_SIGNED (e) \ ? ~ _GL_SIGNED_INT_MAXIMUM (e) \ : _GL_INT_CONVERT (e, 0)) #define _GL_INT_MAXIMUM(e) \ (EXPR_SIGNED (e) \ ? _GL_SIGNED_INT_MAXIMUM (e) \ : _GL_INT_NEGATE_CONVERT (e, 1)) #define _GL_SIGNED_INT_MAXIMUM(e) \ (((_GL_INT_CONVERT (e, 1) << (TYPE_WIDTH ((e) + 0) - 2)) - 1) * 2 + 1) /* Work around OpenVMS incompatibility with C99. */ #if !defined LLONG_MAX && defined __INT64_MAX # define LLONG_MAX __INT64_MAX # define LLONG_MIN __INT64_MIN #endif /* This include file assumes that signed types are two's complement without padding bits; the above macros have undefined behavior otherwise. If this is a problem for you, please let us know how to fix it for your host. As a sanity check, test the assumption for some signed types that bounds. */ verify (TYPE_MINIMUM (signed char) == SCHAR_MIN); verify (TYPE_MAXIMUM (signed char) == SCHAR_MAX); verify (TYPE_MINIMUM (short int) == SHRT_MIN); verify (TYPE_MAXIMUM (short int) == SHRT_MAX); verify (TYPE_MINIMUM (int) == INT_MIN); verify (TYPE_MAXIMUM (int) == INT_MAX); verify (TYPE_MINIMUM (long int) == LONG_MIN); verify (TYPE_MAXIMUM (long int) == LONG_MAX); #ifdef LLONG_MAX verify (TYPE_MINIMUM (long long int) == LLONG_MIN); verify (TYPE_MAXIMUM (long long int) == LLONG_MAX); #endif /* Similarly, sanity-check one ISO/IEC TS 18661-1:2014 macro if defined. */ #ifdef UINT_WIDTH verify (TYPE_WIDTH (unsigned int) == UINT_WIDTH); #endif /* Does the __typeof__ keyword work? This could be done by 'configure', but for now it's easier to do it by hand. */ #if (2 <= __GNUC__ || defined __IBM__TYPEOF__ \ || (0x5110 <= __SUNPRO_C && !__STDC__)) # define _GL_HAVE___TYPEOF__ 1 #else # define _GL_HAVE___TYPEOF__ 0 #endif /* Return 1 if the integer type or expression T might be signed. Return 0 if it is definitely unsigned. This macro does not evaluate its argument, and expands to an integer constant expression. */ #if _GL_HAVE___TYPEOF__ # define _GL_SIGNED_TYPE_OR_EXPR(t) TYPE_SIGNED (__typeof__ (t)) #else # define _GL_SIGNED_TYPE_OR_EXPR(t) 1 #endif /* Bound on length of the string representing an unsigned integer value representable in B bits. log10 (2.0) < 146/485. The smallest value of B where this bound is not tight is 2621. */ #define INT_BITS_STRLEN_BOUND(b) (((b) * 146 + 484) / 485) /* Bound on length of the string representing an integer type or expression T. Subtract 1 for the sign bit if T is signed, and then add 1 more for a minus sign if needed. Because _GL_SIGNED_TYPE_OR_EXPR sometimes returns 0 when its argument is signed, this macro may overestimate the true bound by one byte when applied to unsigned types of size 2, 4, 16, ... bytes. */ #define INT_STRLEN_BOUND(t) \ (INT_BITS_STRLEN_BOUND (TYPE_WIDTH (t) - _GL_SIGNED_TYPE_OR_EXPR (t)) \ + _GL_SIGNED_TYPE_OR_EXPR (t)) /* Bound on buffer size needed to represent an integer type or expression T, including the terminating null. */ #define INT_BUFSIZE_BOUND(t) (INT_STRLEN_BOUND (t) + 1) /* Range overflow checks. The INT__RANGE_OVERFLOW macros return 1 if the corresponding C operators might not yield numerically correct answers due to arithmetic overflow. They do not rely on undefined or implementation-defined behavior. Their implementations are simple and straightforward, but they are a bit harder to use than the INT__OVERFLOW macros described below. Example usage: long int i = ...; long int j = ...; if (INT_MULTIPLY_RANGE_OVERFLOW (i, j, LONG_MIN, LONG_MAX)) printf ("multiply would overflow"); else printf ("product is %ld", i * j); Restrictions on *_RANGE_OVERFLOW macros: These macros do not check for all possible numerical problems or undefined or unspecified behavior: they do not check for division by zero, for bad shift counts, or for shifting negative numbers. These macros may evaluate their arguments zero or multiple times, so the arguments should not have side effects. The arithmetic arguments (including the MIN and MAX arguments) must be of the same integer type after the usual arithmetic conversions, and the type must have minimum value MIN and maximum MAX. Unsigned types should use a zero MIN of the proper type. These macros are tuned for constant MIN and MAX. For commutative operations such as A + B, they are also tuned for constant B. */ /* Return 1 if A + B would overflow in [MIN,MAX] arithmetic. See above for restrictions. */ #define INT_ADD_RANGE_OVERFLOW(a, b, min, max) \ ((b) < 0 \ ? (a) < (min) - (b) \ : (max) - (b) < (a)) /* Return 1 if A - B would overflow in [MIN,MAX] arithmetic. See above for restrictions. */ #define INT_SUBTRACT_RANGE_OVERFLOW(a, b, min, max) \ ((b) < 0 \ ? (max) + (b) < (a) \ : (a) < (min) + (b)) /* Return 1 if - A would overflow in [MIN,MAX] arithmetic. See above for restrictions. */ #define INT_NEGATE_RANGE_OVERFLOW(a, min, max) \ ((min) < 0 \ ? (a) < - (max) \ : 0 < (a)) /* Return 1 if A * B would overflow in [MIN,MAX] arithmetic. See above for restrictions. Avoid && and || as they tickle bugs in Sun C 5.11 2010/08/13 and other compilers; see . */ #define INT_MULTIPLY_RANGE_OVERFLOW(a, b, min, max) \ ((b) < 0 \ ? ((a) < 0 \ ? (a) < (max) / (b) \ : (b) == -1 \ ? 0 \ : (min) / (b) < (a)) \ : (b) == 0 \ ? 0 \ : ((a) < 0 \ ? (a) < (min) / (b) \ : (max) / (b) < (a))) /* Return 1 if A / B would overflow in [MIN,MAX] arithmetic. See above for restrictions. Do not check for division by zero. */ #define INT_DIVIDE_RANGE_OVERFLOW(a, b, min, max) \ ((min) < 0 && (b) == -1 && (a) < - (max)) /* Return 1 if A % B would overflow in [MIN,MAX] arithmetic. See above for restrictions. Do not check for division by zero. Mathematically, % should never overflow, but on x86-like hosts INT_MIN % -1 traps, and the C standard permits this, so treat this as an overflow too. */ #define INT_REMAINDER_RANGE_OVERFLOW(a, b, min, max) \ INT_DIVIDE_RANGE_OVERFLOW (a, b, min, max) /* Return 1 if A << B would overflow in [MIN,MAX] arithmetic. See above for restrictions. Here, MIN and MAX are for A only, and B need not be of the same type as the other arguments. The C standard says that behavior is undefined for shifts unless 0 <= B < wordwidth, and that when A is negative then A << B has undefined behavior and A >> B has implementation-defined behavior, but do not check these other restrictions. */ #define INT_LEFT_SHIFT_RANGE_OVERFLOW(a, b, min, max) \ ((a) < 0 \ ? (a) < (min) >> (b) \ : (max) >> (b) < (a)) /* True if __builtin_add_overflow (A, B, P) works when P is non-null. */ #define _GL_HAS_BUILTIN_OVERFLOW \ (5 <= __GNUC__ || __has_builtin (__builtin_add_overflow)) /* True if __builtin_add_overflow_p (A, B, C) works. */ #define _GL_HAS_BUILTIN_OVERFLOW_P \ (7 <= __GNUC__ || __has_builtin (__builtin_add_overflow_p)) /* The _GL*_OVERFLOW macros have the same restrictions as the *_RANGE_OVERFLOW macros, except that they do not assume that operands (e.g., A and B) have the same type as MIN and MAX. Instead, they assume that the result (e.g., A + B) has that type. */ #if _GL_HAS_BUILTIN_OVERFLOW_P # define _GL_ADD_OVERFLOW(a, b, min, max) \ __builtin_add_overflow_p (a, b, (__typeof__ ((a) + (b))) 0) # define _GL_SUBTRACT_OVERFLOW(a, b, min, max) \ __builtin_sub_overflow_p (a, b, (__typeof__ ((a) - (b))) 0) # define _GL_MULTIPLY_OVERFLOW(a, b, min, max) \ __builtin_mul_overflow_p (a, b, (__typeof__ ((a) * (b))) 0) #else # define _GL_ADD_OVERFLOW(a, b, min, max) \ ((min) < 0 ? INT_ADD_RANGE_OVERFLOW (a, b, min, max) \ : (a) < 0 ? (b) <= (a) + (b) \ : (b) < 0 ? (a) <= (a) + (b) \ : (a) + (b) < (b)) # define _GL_SUBTRACT_OVERFLOW(a, b, min, max) \ ((min) < 0 ? INT_SUBTRACT_RANGE_OVERFLOW (a, b, min, max) \ : (a) < 0 ? 1 \ : (b) < 0 ? (a) - (b) <= (a) \ : (a) < (b)) # define _GL_MULTIPLY_OVERFLOW(a, b, min, max) \ (((min) == 0 && (((a) < 0 && 0 < (b)) || ((b) < 0 && 0 < (a)))) \ || INT_MULTIPLY_RANGE_OVERFLOW (a, b, min, max)) #endif #define _GL_DIVIDE_OVERFLOW(a, b, min, max) \ ((min) < 0 ? (b) == _GL_INT_NEGATE_CONVERT (min, 1) && (a) < - (max) \ : (a) < 0 ? (b) <= (a) + (b) - 1 \ : (b) < 0 && (a) + (b) <= (a)) #define _GL_REMAINDER_OVERFLOW(a, b, min, max) \ ((min) < 0 ? (b) == _GL_INT_NEGATE_CONVERT (min, 1) && (a) < - (max) \ : (a) < 0 ? (a) % (b) != ((max) - (b) + 1) % (b) \ : (b) < 0 && ! _GL_UNSIGNED_NEG_MULTIPLE (a, b, max)) /* Return a nonzero value if A is a mathematical multiple of B, where A is unsigned, B is negative, and MAX is the maximum value of A's type. A's type must be the same as (A % B)'s type. Normally (A % -B == 0) suffices, but things get tricky if -B would overflow. */ #define _GL_UNSIGNED_NEG_MULTIPLE(a, b, max) \ (((b) < -_GL_SIGNED_INT_MAXIMUM (b) \ ? (_GL_SIGNED_INT_MAXIMUM (b) == (max) \ ? (a) \ : (a) % (_GL_INT_CONVERT (a, _GL_SIGNED_INT_MAXIMUM (b)) + 1)) \ : (a) % - (b)) \ == 0) /* Check for integer overflow, and report low order bits of answer. The INT__OVERFLOW macros return 1 if the corresponding C operators might not yield numerically correct answers due to arithmetic overflow. The INT__WRAPV macros also store the low-order bits of the answer. These macros work correctly on all known practical hosts, and do not rely on undefined behavior due to signed arithmetic overflow. Example usage, assuming A and B are long int: if (INT_MULTIPLY_OVERFLOW (a, b)) printf ("result would overflow\n"); else printf ("result is %ld (no overflow)\n", a * b); Example usage with WRAPV flavor: long int result; bool overflow = INT_MULTIPLY_WRAPV (a, b, &result); printf ("result is %ld (%s)\n", result, overflow ? "after overflow" : "no overflow"); Restrictions on these macros: These macros do not check for all possible numerical problems or undefined or unspecified behavior: they do not check for division by zero, for bad shift counts, or for shifting negative numbers. These macros may evaluate their arguments zero or multiple times, so the arguments should not have side effects. The WRAPV macros are not constant expressions. They support only +, binary -, and *. The result type must be signed. These macros are tuned for their last argument being a constant. Return 1 if the integer expressions A * B, A - B, -A, A * B, A / B, A % B, and A << B would overflow, respectively. */ #define INT_ADD_OVERFLOW(a, b) \ _GL_BINARY_OP_OVERFLOW (a, b, _GL_ADD_OVERFLOW) #define INT_SUBTRACT_OVERFLOW(a, b) \ _GL_BINARY_OP_OVERFLOW (a, b, _GL_SUBTRACT_OVERFLOW) #if _GL_HAS_BUILTIN_OVERFLOW_P # define INT_NEGATE_OVERFLOW(a) INT_SUBTRACT_OVERFLOW (0, a) #else # define INT_NEGATE_OVERFLOW(a) \ INT_NEGATE_RANGE_OVERFLOW (a, _GL_INT_MINIMUM (a), _GL_INT_MAXIMUM (a)) #endif #define INT_MULTIPLY_OVERFLOW(a, b) \ _GL_BINARY_OP_OVERFLOW (a, b, _GL_MULTIPLY_OVERFLOW) #define INT_DIVIDE_OVERFLOW(a, b) \ _GL_BINARY_OP_OVERFLOW (a, b, _GL_DIVIDE_OVERFLOW) #define INT_REMAINDER_OVERFLOW(a, b) \ _GL_BINARY_OP_OVERFLOW (a, b, _GL_REMAINDER_OVERFLOW) #define INT_LEFT_SHIFT_OVERFLOW(a, b) \ INT_LEFT_SHIFT_RANGE_OVERFLOW (a, b, \ _GL_INT_MINIMUM (a), _GL_INT_MAXIMUM (a)) /* Return 1 if the expression A B would overflow, where OP_RESULT_OVERFLOW (A, B, MIN, MAX) does the actual test, assuming MIN and MAX are the minimum and maximum for the result type. Arguments should be free of side effects. */ #define _GL_BINARY_OP_OVERFLOW(a, b, op_result_overflow) \ op_result_overflow (a, b, \ _GL_INT_MINIMUM (0 * (b) + (a)), \ _GL_INT_MAXIMUM (0 * (b) + (a))) /* Store the low-order bits of A + B, A - B, A * B, respectively, into *R. Return 1 if the result overflows. See above for restrictions. */ #define INT_ADD_WRAPV(a, b, r) \ _GL_INT_OP_WRAPV (a, b, r, +, __builtin_add_overflow, INT_ADD_OVERFLOW) #define INT_SUBTRACT_WRAPV(a, b, r) \ _GL_INT_OP_WRAPV (a, b, r, -, __builtin_sub_overflow, INT_SUBTRACT_OVERFLOW) #define INT_MULTIPLY_WRAPV(a, b, r) \ _GL_INT_OP_WRAPV (a, b, r, *, __builtin_mul_overflow, INT_MULTIPLY_OVERFLOW) /* Nonzero if this compiler has GCC bug 68193 or Clang bug 25390. See: https://gcc.gnu.org/bugzilla/show_bug.cgi?id=68193 https://llvm.org/bugs/show_bug.cgi?id=25390 For now, assume all versions of GCC-like compilers generate bogus warnings for _Generic. This matters only for older compilers that lack __builtin_add_overflow. */ #if __GNUC__ # define _GL__GENERIC_BOGUS 1 #else # define _GL__GENERIC_BOGUS 0 #endif /* Store the low-order bits of A B into *R, where OP specifies the operation. BUILTIN is the builtin operation, and OVERFLOW the overflow predicate. Return 1 if the result overflows. See above for restrictions. */ #if _GL_HAS_BUILTIN_OVERFLOW # define _GL_INT_OP_WRAPV(a, b, r, op, builtin, overflow) builtin (a, b, r) #elif 201112 <= __STDC_VERSION__ && !_GL__GENERIC_BOGUS # define _GL_INT_OP_WRAPV(a, b, r, op, builtin, overflow) \ (_Generic \ (*(r), \ signed char: \ _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned char, \ signed char, SCHAR_MIN, SCHAR_MAX), \ short int: \ _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned short int, \ short int, SHRT_MIN, SHRT_MAX), \ int: \ _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned int, \ int, INT_MIN, INT_MAX), \ long int: \ _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned long int, \ long int, LONG_MIN, LONG_MAX), \ long long int: \ _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned long long int, \ long long int, LLONG_MIN, LLONG_MAX))) #else # define _GL_INT_OP_WRAPV(a, b, r, op, builtin, overflow) \ (sizeof *(r) == sizeof (signed char) \ ? _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned char, \ signed char, SCHAR_MIN, SCHAR_MAX) \ : sizeof *(r) == sizeof (short int) \ ? _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned short int, \ short int, SHRT_MIN, SHRT_MAX) \ : sizeof *(r) == sizeof (int) \ ? _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned int, \ int, INT_MIN, INT_MAX) \ : _GL_INT_OP_WRAPV_LONGISH(a, b, r, op, overflow)) # ifdef LLONG_MAX # define _GL_INT_OP_WRAPV_LONGISH(a, b, r, op, overflow) \ (sizeof *(r) == sizeof (long int) \ ? _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned long int, \ long int, LONG_MIN, LONG_MAX) \ : _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned long long int, \ long long int, LLONG_MIN, LLONG_MAX)) # else # define _GL_INT_OP_WRAPV_LONGISH(a, b, r, op, overflow) \ _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned long int, \ long int, LONG_MIN, LONG_MAX) # endif #endif /* Store the low-order bits of A B into *R, where the operation is given by OP. Use the unsigned type UT for calculation to avoid overflow problems. *R's type is T, with extremal values TMIN and TMAX. T must be a signed integer type. Return 1 if the result overflows. */ #define _GL_INT_OP_CALC(a, b, r, op, overflow, ut, t, tmin, tmax) \ (sizeof ((a) op (b)) < sizeof (t) \ ? _GL_INT_OP_CALC1 ((t) (a), (t) (b), r, op, overflow, ut, t, tmin, tmax) \ : _GL_INT_OP_CALC1 (a, b, r, op, overflow, ut, t, tmin, tmax)) #define _GL_INT_OP_CALC1(a, b, r, op, overflow, ut, t, tmin, tmax) \ ((overflow (a, b) \ || (EXPR_SIGNED ((a) op (b)) && ((a) op (b)) < (tmin)) \ || (tmax) < ((a) op (b))) \ ? (*(r) = _GL_INT_OP_WRAPV_VIA_UNSIGNED (a, b, op, ut, t, tmin, tmax), 1) \ : (*(r) = _GL_INT_OP_WRAPV_VIA_UNSIGNED (a, b, op, ut, t, tmin, tmax), 0)) /* Return A B, where the operation is given by OP. Use the unsigned type UT for calculation to avoid overflow problems. Convert the result to type T without overflow by subtracting TMIN from large values before converting, and adding it afterwards. Compilers can optimize all the operations except OP. */ #define _GL_INT_OP_WRAPV_VIA_UNSIGNED(a, b, op, ut, t, tmin, tmax) \ (((ut) (a) op (ut) (b)) <= (tmax) \ ? (t) ((ut) (a) op (ut) (b)) \ : ((t) (((ut) (a) op (ut) (b)) - (tmin)) + (tmin))) #endif /* _GL_INTPROPS_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/hard-locale.h0000644000175000017500000000157113004436754016727 00000000000000/* Determine whether a locale is hard. Copyright (C) 1999, 2003-2004, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef HARD_LOCALE_H_ # define HARD_LOCALE_H_ 1 # include bool hard_locale (int); #endif /* HARD_LOCALE_H_ */ gnuastro-0.2.33-8a3b/bootstrapped/lib/getopt_int.h0000644000175000017500000001174213004436754016731 00000000000000/* Internal declarations for getopt. Copyright (C) 1989-1994, 1996-1999, 2001, 2003-2004, 2009-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _GETOPT_INT_H #define _GETOPT_INT_H 1 #include extern int _getopt_internal (int ___argc, char **___argv, const char *__shortopts, const struct option *__longopts, int *__longind, int __long_only, int __posixly_correct); /* Reentrant versions which can handle parsing multiple argument vectors at the same time. */ /* Describe how to deal with options that follow non-option ARGV-elements. If the caller did not specify anything, the default is REQUIRE_ORDER if the environment variable POSIXLY_CORRECT is defined, PERMUTE otherwise. REQUIRE_ORDER means don't recognize them as options; stop option processing when the first non-option is seen. This is what Unix does. This mode of operation is selected by either setting the environment variable POSIXLY_CORRECT, or using '+' as the first character of the list of option characters, or by calling getopt. PERMUTE is the default. We permute the contents of ARGV as we scan, so that eventually all the non-options are at the end. This allows options to be given in any order, even with programs that were not written to expect this. RETURN_IN_ORDER is an option available to programs that were written to expect options and other ARGV-elements in any order and that care about the ordering of the two. We describe each non-option ARGV-element as if it were the argument of an option with character code 1. Using '-' as the first character of the list of option characters selects this mode of operation. The special argument '--' forces an end of option-scanning regardless of the value of 'ordering'. In the case of RETURN_IN_ORDER, only '--' can cause 'getopt' to return -1 with 'optind' != ARGC. */ enum __ord { REQUIRE_ORDER, PERMUTE, RETURN_IN_ORDER }; /* Data type for reentrant functions. */ struct _getopt_data { /* These have exactly the same meaning as the corresponding global variables, except that they are used for the reentrant versions of getopt. */ int optind; int opterr; int optopt; char *optarg; /* Internal members. */ /* True if the internal members have been initialized. */ int __initialized; /* The next char to be scanned in the option-element in which the last option character we returned was found. This allows us to pick up the scan where we left off. If this is zero, or a null string, it means resume the scan by advancing to the next ARGV-element. */ char *__nextchar; /* See __ord above. */ enum __ord __ordering; /* If the POSIXLY_CORRECT environment variable is set or getopt was called. */ int __posixly_correct; /* Handle permutation of arguments. */ /* Describe the part of ARGV that contains non-options that have been skipped. 'first_nonopt' is the index in ARGV of the first of them; 'last_nonopt' is the index after the last of them. */ int __first_nonopt; int __last_nonopt; #if defined _LIBC && defined USE_NONOPTION_FLAGS int __nonoption_flags_max_len; int __nonoption_flags_len; #endif }; /* The initializer is necessary to set OPTIND and OPTERR to their default values and to clear the initialization flag. */ #define _GETOPT_DATA_INITIALIZER { 1, 1 } extern int _getopt_internal_r (int ___argc, char **___argv, const char *__shortopts, const struct option *__longopts, int *__longind, int __long_only, struct _getopt_data *__data, int __posixly_correct); extern int _getopt_long_r (int ___argc, char **___argv, const char *__shortopts, const struct option *__longopts, int *__longind, struct _getopt_data *__data); extern int _getopt_long_only_r (int ___argc, char **___argv, const char *__shortopts, const struct option *__longopts, int *__longind, struct _getopt_data *__data); #endif /* getopt_int.h */ gnuastro-0.2.33-8a3b/bootstrapped/lib/getopt.in.h0000644000175000017500000002162113004436754016461 00000000000000/* Declarations for getopt. Copyright (C) 1989-1994, 1996-1999, 2001, 2003-2007, 2009-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _@GUARD_PREFIX@_GETOPT_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* The include_next requires a split double-inclusion guard. We must also inform the replacement unistd.h to not recursively use ; our definitions will be present soon enough. */ #if @HAVE_GETOPT_H@ # define _GL_SYSTEM_GETOPT # @INCLUDE_NEXT@ @NEXT_GETOPT_H@ # undef _GL_SYSTEM_GETOPT #endif #ifndef _@GUARD_PREFIX@_GETOPT_H #ifndef __need_getopt # define _@GUARD_PREFIX@_GETOPT_H 1 #endif /* Standalone applications should #define __GETOPT_PREFIX to an identifier that prefixes the external functions and variables defined in this header. When this happens, include the headers that might declare getopt so that they will not cause confusion if included after this file (if the system had , we have already included it). Then systematically rename identifiers so that they do not collide with the system functions and variables. Renaming avoids problems with some compilers and linkers. */ #if defined __GETOPT_PREFIX && !defined __need_getopt # if !@HAVE_GETOPT_H@ # define __need_system_stdlib_h # include # undef __need_system_stdlib_h # include # include # endif # undef __need_getopt # undef getopt # undef getopt_long # undef getopt_long_only # undef optarg # undef opterr # undef optind # undef optopt # undef option # define __GETOPT_CONCAT(x, y) x ## y # define __GETOPT_XCONCAT(x, y) __GETOPT_CONCAT (x, y) # define __GETOPT_ID(y) __GETOPT_XCONCAT (__GETOPT_PREFIX, y) # define getopt __GETOPT_ID (getopt) # define getopt_long __GETOPT_ID (getopt_long) # define getopt_long_only __GETOPT_ID (getopt_long_only) # define optarg __GETOPT_ID (optarg) # define opterr __GETOPT_ID (opterr) # define optind __GETOPT_ID (optind) # define optopt __GETOPT_ID (optopt) # define option __GETOPT_ID (option) # define _getopt_internal __GETOPT_ID (getopt_internal) #endif /* Standalone applications get correct prototypes for getopt_long and getopt_long_only; they declare "char **argv". libc uses prototypes with "char *const *argv" that are incorrect because getopt_long and getopt_long_only can permute argv; this is required for backward compatibility (e.g., for LSB 2.0.1). This used to be '#if defined __GETOPT_PREFIX && !defined __need_getopt', but it caused redefinition warnings if both unistd.h and getopt.h were included, since unistd.h includes getopt.h having previously defined __need_getopt. The only place where __getopt_argv_const is used is in definitions of getopt_long and getopt_long_only below, but these are visible only if __need_getopt is not defined, so it is quite safe to rewrite the conditional as follows: */ #if !defined __need_getopt # if defined __GETOPT_PREFIX # define __getopt_argv_const /* empty */ # else # define __getopt_argv_const const # endif #endif /* If __GNU_LIBRARY__ is not already defined, either we are being used standalone, or this is the first header included in the source file. If we are being used with glibc, we need to include , but that does not exist if we are standalone. So: if __GNU_LIBRARY__ is not defined, include , which will pull in for us if it's from glibc. (Why ctype.h? It's guaranteed to exist and it doesn't flood the namespace with stuff the way some other headers do.) */ #if !defined __GNU_LIBRARY__ # include #endif #ifndef __THROW # ifndef __GNUC_PREREQ # define __GNUC_PREREQ(maj, min) (0) # endif # if defined __cplusplus && __GNUC_PREREQ (2,8) # define __THROW throw () # else # define __THROW # endif #endif /* The definition of _GL_ARG_NONNULL is copied here. */ #ifdef __cplusplus extern "C" { #endif /* For communication from 'getopt' to the caller. When 'getopt' finds an option that takes an argument, the argument value is returned here. Also, when 'ordering' is RETURN_IN_ORDER, each non-option ARGV-element is returned here. */ extern char *optarg; /* Index in ARGV of the next element to be scanned. This is used for communication to and from the caller and for communication between successive calls to 'getopt'. On entry to 'getopt', zero means this is the first call; initialize. When 'getopt' returns -1, this is the index of the first of the non-option elements that the caller should itself scan. Otherwise, 'optind' communicates from one call to the next how much of ARGV has been scanned so far. */ extern int optind; /* Callers store zero here to inhibit the error message 'getopt' prints for unrecognized options. */ extern int opterr; /* Set to an option character which was unrecognized. */ extern int optopt; #ifndef __need_getopt /* Describe the long-named options requested by the application. The LONG_OPTIONS argument to getopt_long or getopt_long_only is a vector of 'struct option' terminated by an element containing a name which is zero. The field 'has_arg' is: no_argument (or 0) if the option does not take an argument, required_argument (or 1) if the option requires an argument, optional_argument (or 2) if the option takes an optional argument. If the field 'flag' is not NULL, it points to a variable that is set to the value given in the field 'val' when the option is found, but left unchanged if the option is not found. To have a long-named option do something other than set an 'int' to a compiled-in constant, such as set a value from 'optarg', set the option's 'flag' field to zero and its 'val' field to a nonzero value (the equivalent single-letter option character, if there is one). For long options that have a zero 'flag' field, 'getopt' returns the contents of the 'val' field. */ # if !GNULIB_defined_struct_option struct option { const char *name; /* has_arg can't be an enum because some compilers complain about type mismatches in all the code that assumes it is an int. */ int has_arg; int *flag; int val; }; # define GNULIB_defined_struct_option 1 # endif /* Names for the values of the 'has_arg' field of 'struct option'. */ # define no_argument 0 # define required_argument 1 # define optional_argument 2 #endif /* need getopt */ /* Get definitions and prototypes for functions to process the arguments in ARGV (ARGC of them, minus the program name) for options given in OPTS. Return the option character from OPTS just read. Return -1 when there are no more options. For unrecognized options, or options missing arguments, 'optopt' is set to the option letter, and '?' is returned. The OPTS string is a list of characters which are recognized option letters, optionally followed by colons, specifying that that letter takes an argument, to be placed in 'optarg'. If a letter in OPTS is followed by two colons, its argument is optional. This behavior is specific to the GNU 'getopt'. The argument '--' causes premature termination of argument scanning, explicitly telling 'getopt' that there are no more options. If OPTS begins with '-', then non-option arguments are treated as arguments to the option '\1'. This behavior is specific to the GNU 'getopt'. If OPTS begins with '+', or POSIXLY_CORRECT is set in the environment, then do not permute arguments. */ extern int getopt (int ___argc, char *const *___argv, const char *__shortopts) __THROW _GL_ARG_NONNULL ((2, 3)); #ifndef __need_getopt extern int getopt_long (int ___argc, char *__getopt_argv_const *___argv, const char *__shortopts, const struct option *__longopts, int *__longind) __THROW _GL_ARG_NONNULL ((2, 3)); extern int getopt_long_only (int ___argc, char *__getopt_argv_const *___argv, const char *__shortopts, const struct option *__longopts, int *__longind) __THROW _GL_ARG_NONNULL ((2, 3)); #endif #ifdef __cplusplus } #endif /* Make sure we later can get all the definitions and declarations. */ #undef __need_getopt #endif /* _@GUARD_PREFIX@_GETOPT_H */ #endif /* _@GUARD_PREFIX@_GETOPT_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/float.in.h0000644000175000017500000001673413004436754016275 00000000000000/* A correct . Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _@GUARD_PREFIX@_FLOAT_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_FLOAT_H@ #ifndef _@GUARD_PREFIX@_FLOAT_H #define _@GUARD_PREFIX@_FLOAT_H /* 'long double' properties. */ #if defined __i386__ && (defined __BEOS__ || defined __OpenBSD__) /* Number of mantissa units, in base FLT_RADIX. */ # undef LDBL_MANT_DIG # define LDBL_MANT_DIG 64 /* Number of decimal digits that is sufficient for representing a number. */ # undef LDBL_DIG # define LDBL_DIG 18 /* x-1 where x is the smallest representable number > 1. */ # undef LDBL_EPSILON # define LDBL_EPSILON 1.0842021724855044340E-19L /* Minimum e such that FLT_RADIX^(e-1) is a normalized number. */ # undef LDBL_MIN_EXP # define LDBL_MIN_EXP (-16381) /* Maximum e such that FLT_RADIX^(e-1) is a representable finite number. */ # undef LDBL_MAX_EXP # define LDBL_MAX_EXP 16384 /* Minimum positive normalized number. */ # undef LDBL_MIN # define LDBL_MIN 3.3621031431120935063E-4932L /* Maximum representable finite number. */ # undef LDBL_MAX # define LDBL_MAX 1.1897314953572317650E+4932L /* Minimum e such that 10^e is in the range of normalized numbers. */ # undef LDBL_MIN_10_EXP # define LDBL_MIN_10_EXP (-4931) /* Maximum e such that 10^e is in the range of representable finite numbers. */ # undef LDBL_MAX_10_EXP # define LDBL_MAX_10_EXP 4932 #endif /* On FreeBSD/x86 6.4, the 'long double' type really has only 53 bits of precision in the compiler but 64 bits of precision at runtime. See . */ #if defined __i386__ && defined __FreeBSD__ /* Number of mantissa units, in base FLT_RADIX. */ # undef LDBL_MANT_DIG # define LDBL_MANT_DIG 64 /* Number of decimal digits that is sufficient for representing a number. */ # undef LDBL_DIG # define LDBL_DIG 18 /* x-1 where x is the smallest representable number > 1. */ # undef LDBL_EPSILON # define LDBL_EPSILON 1.084202172485504434007452800869941711426e-19L /* 2^-63 */ /* Minimum e such that FLT_RADIX^(e-1) is a normalized number. */ # undef LDBL_MIN_EXP # define LDBL_MIN_EXP (-16381) /* Maximum e such that FLT_RADIX^(e-1) is a representable finite number. */ # undef LDBL_MAX_EXP # define LDBL_MAX_EXP 16384 /* Minimum positive normalized number. */ # undef LDBL_MIN # define LDBL_MIN 3.3621031431120935E-4932L /* = 0x1p-16382L */ /* Maximum representable finite number. */ # undef LDBL_MAX /* LDBL_MAX is represented as { 0xFFFFFFFF, 0xFFFFFFFF, 32766 }. But the largest literal that GCC allows us to write is 0x0.fffffffffffff8p16384L = { 0xFFFFF800, 0xFFFFFFFF, 32766 }. So, define it like this through a reference to an external variable const unsigned int LDBL_MAX[3] = { 0xFFFFFFFF, 0xFFFFFFFF, 32766 }; extern const long double LDBL_MAX; Unfortunately, this is not a constant expression. */ union gl_long_double_union { struct { unsigned int lo; unsigned int hi; unsigned int exponent; } xd; long double ld; }; extern const union gl_long_double_union gl_LDBL_MAX; # define LDBL_MAX (gl_LDBL_MAX.ld) /* Minimum e such that 10^e is in the range of normalized numbers. */ # undef LDBL_MIN_10_EXP # define LDBL_MIN_10_EXP (-4931) /* Maximum e such that 10^e is in the range of representable finite numbers. */ # undef LDBL_MAX_10_EXP # define LDBL_MAX_10_EXP 4932 #endif /* On AIX 7.1 with gcc 4.2, the values of LDBL_MIN_EXP, LDBL_MIN, LDBL_MAX are wrong. On Linux/PowerPC with gcc 4.4, the value of LDBL_MAX is wrong. */ #if (defined _ARCH_PPC || defined _POWER) && defined _AIX && (LDBL_MANT_DIG == 106) && defined __GNUC__ # undef LDBL_MIN_EXP # define LDBL_MIN_EXP DBL_MIN_EXP # undef LDBL_MIN_10_EXP # define LDBL_MIN_10_EXP DBL_MIN_10_EXP # undef LDBL_MIN # define LDBL_MIN 2.22507385850720138309023271733240406422e-308L /* DBL_MIN = 2^-1022 */ #endif #if (defined _ARCH_PPC || defined _POWER) && (defined _AIX || defined __linux__) && (LDBL_MANT_DIG == 106) && defined __GNUC__ # undef LDBL_MAX /* LDBL_MAX is represented as { 0x7FEFFFFF, 0xFFFFFFFF, 0x7C8FFFFF, 0xFFFFFFFF }. It is not easy to define: #define LDBL_MAX 1.79769313486231580793728971405302307166e308L is too small, whereas #define LDBL_MAX 1.79769313486231580793728971405302307167e308L is too large. Apparently a bug in GCC decimal-to-binary conversion. Also, I can't get values larger than #define LDBL63 ((long double) (1ULL << 63)) #define LDBL882 (LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63) #define LDBL945 (LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63) #define LDBL1008 (LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63) #define LDBL_MAX (LDBL1008 * 65535.0L + LDBL945 * (long double) 9223372036821221375ULL + LDBL882 * (long double) 4611686018427387904ULL) which is represented as { 0x7FEFFFFF, 0xFFFFFFFF, 0x7C8FFFFF, 0xF8000000 }. So, define it like this through a reference to an external variable const double LDBL_MAX[2] = { DBL_MAX, DBL_MAX / (double)134217728UL / (double)134217728UL }; extern const long double LDBL_MAX; or through a pointer cast #define LDBL_MAX \ (*(const long double *) (double[]) { DBL_MAX, DBL_MAX / (double)134217728UL / (double)134217728UL }) Unfortunately, this is not a constant expression, and the latter expression does not work well when GCC is optimizing.. */ union gl_long_double_union { struct { double hi; double lo; } dd; long double ld; }; extern const union gl_long_double_union gl_LDBL_MAX; # define LDBL_MAX (gl_LDBL_MAX.ld) #endif /* On IRIX 6.5, with cc, the value of LDBL_MANT_DIG is wrong. On IRIX 6.5, with gcc 4.2, the values of LDBL_MIN_EXP, LDBL_MIN, LDBL_EPSILON are wrong. */ #if defined __sgi && (LDBL_MANT_DIG >= 106) # undef LDBL_MANT_DIG # define LDBL_MANT_DIG 106 # if defined __GNUC__ # undef LDBL_MIN_EXP # define LDBL_MIN_EXP DBL_MIN_EXP # undef LDBL_MIN_10_EXP # define LDBL_MIN_10_EXP DBL_MIN_10_EXP # undef LDBL_MIN # define LDBL_MIN 2.22507385850720138309023271733240406422e-308L /* DBL_MIN = 2^-1022 */ # undef LDBL_EPSILON # define LDBL_EPSILON 2.46519032881566189191165176650870696773e-32L /* 2^-105 */ # endif #endif #if @REPLACE_ITOLD@ /* Pull in a function that fixes the 'int' to 'long double' conversion of glibc 2.7. */ extern # ifdef __cplusplus "C" # endif void _Qp_itoq (long double *, int); static void (*_gl_float_fix_itold) (long double *, int) = _Qp_itoq; #endif #endif /* _@GUARD_PREFIX@_FLOAT_H */ #endif /* _@GUARD_PREFIX@_FLOAT_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/error.h0000644000175000017500000000553213004436754015706 00000000000000/* Declaration for error-reporting function Copyright (C) 1995-1997, 2003, 2006, 2008-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _ERROR_H #define _ERROR_H 1 /* The __attribute__ feature is available in gcc versions 2.5 and later. The __-protected variants of the attributes 'format' and 'printf' are accepted by gcc versions 2.6.4 (effectively 2.7) and later. We enable _GL_ATTRIBUTE_FORMAT only if these are supported too, because gnulib and libintl do '#define printf __printf__' when they override the 'printf' function. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 7) # define _GL_ATTRIBUTE_FORMAT(spec) __attribute__ ((__format__ spec)) #else # define _GL_ATTRIBUTE_FORMAT(spec) /* empty */ #endif /* On mingw, the flavor of printf depends on whether the extensions module * is in use; the check for determines the witness macro. */ #ifndef _GL_ATTRIBUTE_SPEC_PRINTF # if GNULIB_PRINTF_ATTRIBUTE_FLAVOR_GNU # define _GL_ATTRIBUTE_SPEC_PRINTF __gnu_printf__ # else # define _GL_ATTRIBUTE_SPEC_PRINTF __printf__ # endif #endif #ifdef __cplusplus extern "C" { #endif /* Print a message with 'fprintf (stderr, FORMAT, ...)'; if ERRNUM is nonzero, follow it with ": " and strerror (ERRNUM). If STATUS is nonzero, terminate the program with 'exit (STATUS)'. */ extern void error (int __status, int __errnum, const char *__format, ...) _GL_ATTRIBUTE_FORMAT ((_GL_ATTRIBUTE_SPEC_PRINTF, 3, 4)); extern void error_at_line (int __status, int __errnum, const char *__fname, unsigned int __lineno, const char *__format, ...) _GL_ATTRIBUTE_FORMAT ((_GL_ATTRIBUTE_SPEC_PRINTF, 5, 6)); /* If NULL, error will flush stdout, then print on stderr the program name, a colon and a space. Otherwise, error will call this function without parameters instead. */ extern void (*error_print_progname) (void); /* This variable is incremented each time 'error' is called. */ extern unsigned int error_message_count; /* Sometimes we want to have at most one error per line. This variable controls whether this mode is selected or not. */ extern int error_one_per_line; #ifdef __cplusplus } #endif #endif /* error.h */ gnuastro-0.2.33-8a3b/bootstrapped/lib/errno.in.h0000644000175000017500000001646313004436754016314 00000000000000/* A POSIX-like . Copyright (C) 2008-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _@GUARD_PREFIX@_ERRNO_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_ERRNO_H@ #ifndef _@GUARD_PREFIX@_ERRNO_H #define _@GUARD_PREFIX@_ERRNO_H /* On native Windows platforms, many macros are not defined. */ # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* These are the same values as defined by MSVC 10, for interoperability. */ # ifndef ENOMSG # define ENOMSG 122 # define GNULIB_defined_ENOMSG 1 # endif # ifndef EIDRM # define EIDRM 111 # define GNULIB_defined_EIDRM 1 # endif # ifndef ENOLINK # define ENOLINK 121 # define GNULIB_defined_ENOLINK 1 # endif # ifndef EPROTO # define EPROTO 134 # define GNULIB_defined_EPROTO 1 # endif # ifndef EBADMSG # define EBADMSG 104 # define GNULIB_defined_EBADMSG 1 # endif # ifndef EOVERFLOW # define EOVERFLOW 132 # define GNULIB_defined_EOVERFLOW 1 # endif # ifndef ENOTSUP # define ENOTSUP 129 # define GNULIB_defined_ENOTSUP 1 # endif # ifndef ENETRESET # define ENETRESET 117 # define GNULIB_defined_ENETRESET 1 # endif # ifndef ECONNABORTED # define ECONNABORTED 106 # define GNULIB_defined_ECONNABORTED 1 # endif # ifndef ECANCELED # define ECANCELED 105 # define GNULIB_defined_ECANCELED 1 # endif # ifndef EOWNERDEAD # define EOWNERDEAD 133 # define GNULIB_defined_EOWNERDEAD 1 # endif # ifndef ENOTRECOVERABLE # define ENOTRECOVERABLE 127 # define GNULIB_defined_ENOTRECOVERABLE 1 # endif # ifndef EINPROGRESS # define EINPROGRESS 112 # define EALREADY 103 # define ENOTSOCK 128 # define EDESTADDRREQ 109 # define EMSGSIZE 115 # define EPROTOTYPE 136 # define ENOPROTOOPT 123 # define EPROTONOSUPPORT 135 # define EOPNOTSUPP 130 # define EAFNOSUPPORT 102 # define EADDRINUSE 100 # define EADDRNOTAVAIL 101 # define ENETDOWN 116 # define ENETUNREACH 118 # define ECONNRESET 108 # define ENOBUFS 119 # define EISCONN 113 # define ENOTCONN 126 # define ETIMEDOUT 138 # define ECONNREFUSED 107 # define ELOOP 114 # define EHOSTUNREACH 110 # define EWOULDBLOCK 140 # define GNULIB_defined_ESOCK 1 # endif # ifndef ETXTBSY # define ETXTBSY 139 # define ENODATA 120 /* not required by POSIX */ # define ENOSR 124 /* not required by POSIX */ # define ENOSTR 125 /* not required by POSIX */ # define ETIME 137 /* not required by POSIX */ # define EOTHER 131 /* not required by POSIX */ # define GNULIB_defined_ESTREAMS 1 # endif /* These are intentionally the same values as the WSA* error numbers, defined in . */ # define ESOCKTNOSUPPORT 10044 /* not required by POSIX */ # define EPFNOSUPPORT 10046 /* not required by POSIX */ # define ESHUTDOWN 10058 /* not required by POSIX */ # define ETOOMANYREFS 10059 /* not required by POSIX */ # define EHOSTDOWN 10064 /* not required by POSIX */ # define EPROCLIM 10067 /* not required by POSIX */ # define EUSERS 10068 /* not required by POSIX */ # define EDQUOT 10069 # define ESTALE 10070 # define EREMOTE 10071 /* not required by POSIX */ # define GNULIB_defined_EWINSOCK 1 # endif /* On OSF/1 5.1, when _XOPEN_SOURCE_EXTENDED is not defined, the macros EMULTIHOP, ENOLINK, EOVERFLOW are not defined. */ # if @EMULTIHOP_HIDDEN@ # define EMULTIHOP @EMULTIHOP_VALUE@ # define GNULIB_defined_EMULTIHOP 1 # endif # if @ENOLINK_HIDDEN@ # define ENOLINK @ENOLINK_VALUE@ # define GNULIB_defined_ENOLINK 1 # endif # if @EOVERFLOW_HIDDEN@ # define EOVERFLOW @EOVERFLOW_VALUE@ # define GNULIB_defined_EOVERFLOW 1 # endif /* On OpenBSD 4.0 and on native Windows, the macros ENOMSG, EIDRM, ENOLINK, EPROTO, EMULTIHOP, EBADMSG, EOVERFLOW, ENOTSUP, ECANCELED are not defined. Likewise, on NonStop Kernel, EDQUOT is not defined. Define them here. Values >= 2000 seem safe to use: Solaris ESTALE = 151, HP-UX EWOULDBLOCK = 246, IRIX EDQUOT = 1133. Note: When one of these systems defines some of these macros some day, binaries will have to be recompiled so that they recognizes the new errno values from the system. */ # ifndef ENOMSG # define ENOMSG 2000 # define GNULIB_defined_ENOMSG 1 # endif # ifndef EIDRM # define EIDRM 2001 # define GNULIB_defined_EIDRM 1 # endif # ifndef ENOLINK # define ENOLINK 2002 # define GNULIB_defined_ENOLINK 1 # endif # ifndef EPROTO # define EPROTO 2003 # define GNULIB_defined_EPROTO 1 # endif # ifndef EMULTIHOP # define EMULTIHOP 2004 # define GNULIB_defined_EMULTIHOP 1 # endif # ifndef EBADMSG # define EBADMSG 2005 # define GNULIB_defined_EBADMSG 1 # endif # ifndef EOVERFLOW # define EOVERFLOW 2006 # define GNULIB_defined_EOVERFLOW 1 # endif # ifndef ENOTSUP # define ENOTSUP 2007 # define GNULIB_defined_ENOTSUP 1 # endif # ifndef ENETRESET # define ENETRESET 2011 # define GNULIB_defined_ENETRESET 1 # endif # ifndef ECONNABORTED # define ECONNABORTED 2012 # define GNULIB_defined_ECONNABORTED 1 # endif # ifndef ESTALE # define ESTALE 2009 # define GNULIB_defined_ESTALE 1 # endif # ifndef EDQUOT # define EDQUOT 2010 # define GNULIB_defined_EDQUOT 1 # endif # ifndef ECANCELED # define ECANCELED 2008 # define GNULIB_defined_ECANCELED 1 # endif /* On many platforms, the macros EOWNERDEAD and ENOTRECOVERABLE are not defined. */ # ifndef EOWNERDEAD # if defined __sun /* Use the same values as defined for Solaris >= 8, for interoperability. */ # define EOWNERDEAD 58 # define ENOTRECOVERABLE 59 # elif (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* We have a conflict here: pthreads-win32 defines these values differently than MSVC 10. It's hairy to decide which one to use. */ # if defined __MINGW32__ && !defined USE_WINDOWS_THREADS /* Use the same values as defined by pthreads-win32, for interoperability. */ # define EOWNERDEAD 43 # define ENOTRECOVERABLE 44 # else /* Use the same values as defined by MSVC 10, for interoperability. */ # define EOWNERDEAD 133 # define ENOTRECOVERABLE 127 # endif # else # define EOWNERDEAD 2013 # define ENOTRECOVERABLE 2014 # endif # define GNULIB_defined_EOWNERDEAD 1 # define GNULIB_defined_ENOTRECOVERABLE 1 # endif # ifndef EILSEQ # define EILSEQ 2015 # define GNULIB_defined_EILSEQ 1 # endif #endif /* _@GUARD_PREFIX@_ERRNO_H */ #endif /* _@GUARD_PREFIX@_ERRNO_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/dosname.h0000644000175000017500000000373313004436754016204 00000000000000/* File names on MS-DOS/Windows systems. Copyright (C) 2000-2001, 2004-2006, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . From Paul Eggert and Jim Meyering. */ #ifndef _DOSNAME_H #define _DOSNAME_H #if (defined _WIN32 || defined __WIN32__ || \ defined __MSDOS__ || defined __CYGWIN__ || \ defined __EMX__ || defined __DJGPP__) /* This internal macro assumes ASCII, but all hosts that support drive letters use ASCII. */ # define _IS_DRIVE_LETTER(C) (((unsigned int) (C) | ('a' - 'A')) - 'a' \ <= 'z' - 'a') # define FILE_SYSTEM_PREFIX_LEN(Filename) \ (_IS_DRIVE_LETTER ((Filename)[0]) && (Filename)[1] == ':' ? 2 : 0) # ifndef __CYGWIN__ # define FILE_SYSTEM_DRIVE_PREFIX_CAN_BE_RELATIVE 1 # endif # define ISSLASH(C) ((C) == '/' || (C) == '\\') #else # define FILE_SYSTEM_PREFIX_LEN(Filename) 0 # define ISSLASH(C) ((C) == '/') #endif #ifndef FILE_SYSTEM_DRIVE_PREFIX_CAN_BE_RELATIVE # define FILE_SYSTEM_DRIVE_PREFIX_CAN_BE_RELATIVE 0 #endif #if FILE_SYSTEM_DRIVE_PREFIX_CAN_BE_RELATIVE # define IS_ABSOLUTE_FILE_NAME(F) ISSLASH ((F)[FILE_SYSTEM_PREFIX_LEN (F)]) # else # define IS_ABSOLUTE_FILE_NAME(F) \ (ISSLASH ((F)[0]) || FILE_SYSTEM_PREFIX_LEN (F) != 0) #endif #define IS_RELATIVE_FILE_NAME(F) (! IS_ABSOLUTE_FILE_NAME (F)) #endif /* DOSNAME_H_ */ gnuastro-0.2.33-8a3b/bootstrapped/lib/dirname.h0000644000175000017500000000277713004436754016204 00000000000000/* Take file names apart into directory and base names. Copyright (C) 1998, 2001, 2003-2006, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef DIRNAME_H_ # define DIRNAME_H_ 1 # include # include # include "dosname.h" # ifndef DIRECTORY_SEPARATOR # define DIRECTORY_SEPARATOR '/' # endif # ifndef DOUBLE_SLASH_IS_DISTINCT_ROOT # define DOUBLE_SLASH_IS_DISTINCT_ROOT 0 # endif #ifdef __cplusplus extern "C" { #endif # if GNULIB_DIRNAME char *base_name (char const *file); char *dir_name (char const *file); # endif char *mdir_name (char const *file); size_t base_len (char const *file) _GL_ATTRIBUTE_PURE; size_t dir_len (char const *file) _GL_ATTRIBUTE_PURE; char *last_component (char const *file) _GL_ATTRIBUTE_PURE; bool strip_trailing_slashes (char *file); #ifdef __cplusplus } /* extern "C" */ #endif #endif /* not DIRNAME_H_ */ gnuastro-0.2.33-8a3b/bootstrapped/lib/alloca.in.h0000644000175000017500000000400113004436754016403 00000000000000/* Memory allocation on the stack. Copyright (C) 1995, 1999, 2001-2004, 2006-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Avoid using the symbol _ALLOCA_H here, as Bison assumes _ALLOCA_H means there is a real alloca function. */ #ifndef _GL_ALLOCA_H #define _GL_ALLOCA_H /* alloca (N) returns a pointer to N bytes of memory allocated on the stack, which will last until the function returns. Use of alloca should be avoided: - inside arguments of function calls - undefined behaviour, - in inline functions - the allocation may actually last until the calling function returns, - for huge N (say, N >= 65536) - you never know how large (or small) the stack is, and when the stack cannot fulfill the memory allocation request, the program just crashes. */ #ifndef alloca # ifdef __GNUC__ # define alloca __builtin_alloca # elif defined _AIX # define alloca __alloca # elif defined _MSC_VER # include # define alloca _alloca # elif defined __DECC && defined __VMS # define alloca __ALLOCA # elif defined __TANDEM && defined _TNS_E_TARGET # ifdef __cplusplus extern "C" # endif void *_alloca (unsigned short); # pragma intrinsic (_alloca) # define alloca _alloca # elif defined __MVS__ # include # else # include # ifdef __cplusplus extern "C" # endif void *alloca (size_t); # endif #endif #endif /* _GL_ALLOCA_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/wcrtomb.c0000644000175000017500000000271513004436754016225 00000000000000/* Convert wide character to multibyte character. Copyright (C) 2008-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2008. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include size_t wcrtomb (char *s, wchar_t wc, mbstate_t *ps) { /* This implementation of wcrtomb on top of wctomb() supports only stateless encodings. ps must be in the initial state. */ if (ps != NULL && !mbsinit (ps)) { errno = EINVAL; return (size_t)(-1); } if (s == NULL) /* We know the NUL wide character corresponds to the NUL character. */ return 1; else { int ret = wctomb (s, wc); if (ret >= 0) return ret; else { errno = EILSEQ; return (size_t)(-1); } } } gnuastro-0.2.33-8a3b/bootstrapped/lib/vsnprintf.c0000644000175000017500000000354013004436754016576 00000000000000/* Formatted output to strings. Copyright (C) 2004, 2006-2016 Free Software Foundation, Inc. Written by Simon Josefsson and Yoann Vandoorselaere . This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifdef HAVE_CONFIG_H # include #endif /* Specification. */ #include #include #include #include #include #include #include "vasnprintf.h" /* Print formatted output to string STR. Similar to vsprintf, but additional length SIZE limit how much is written into STR. Returns string length of formatted string (which may be larger than SIZE). STR may be NULL, in which case nothing will be written. On error, return a negative value. */ int vsnprintf (char *str, size_t size, const char *format, va_list args) { char *output; size_t len; size_t lenbuf = size; output = vasnprintf (str, &lenbuf, format, args); len = lenbuf; if (!output) return -1; if (output != str) { if (size) { size_t pruned_len = (len < size ? len : size - 1); memcpy (str, output, pruned_len); str[pruned_len] = '\0'; } free (output); } if (len > INT_MAX) { errno = EOVERFLOW; return -1; } return len; } gnuastro-0.2.33-8a3b/bootstrapped/lib/vasnprintf.c0000644000175000017500000066412713004436754016755 00000000000000/* vsprintf with automatic memory allocation. Copyright (C) 1999, 2002-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* This file can be parametrized with the following macros: VASNPRINTF The name of the function being defined. FCHAR_T The element type of the format string. DCHAR_T The element type of the destination (result) string. FCHAR_T_ONLY_ASCII Set to 1 to enable verification that all characters in the format string are ASCII. MUST be set if FCHAR_T and DCHAR_T are not the same type. DIRECTIVE Structure denoting a format directive. Depends on FCHAR_T. DIRECTIVES Structure denoting the set of format directives of a format string. Depends on FCHAR_T. PRINTF_PARSE Function that parses a format string. Depends on FCHAR_T. DCHAR_CPY memcpy like function for DCHAR_T[] arrays. DCHAR_SET memset like function for DCHAR_T[] arrays. DCHAR_MBSNLEN mbsnlen like function for DCHAR_T[] arrays. SNPRINTF The system's snprintf (or similar) function. This may be either snprintf or swprintf. TCHAR_T The element type of the argument and result string of the said SNPRINTF function. This may be either char or wchar_t. The code exploits that sizeof (TCHAR_T) | sizeof (DCHAR_T) and alignof (TCHAR_T) <= alignof (DCHAR_T). DCHAR_IS_TCHAR Set to 1 if DCHAR_T and TCHAR_T are the same type. DCHAR_CONV_FROM_ENCODING A function to convert from char[] to DCHAR[]. DCHAR_IS_UINT8_T Set to 1 if DCHAR_T is uint8_t. DCHAR_IS_UINT16_T Set to 1 if DCHAR_T is uint16_t. DCHAR_IS_UINT32_T Set to 1 if DCHAR_T is uint32_t. */ /* Tell glibc's to provide a prototype for snprintf(). This must come before because may include , and once has been included, it's too late. */ #ifndef _GNU_SOURCE # define _GNU_SOURCE 1 #endif #ifndef VASNPRINTF # include #endif #ifndef IN_LIBINTL # include #endif /* Specification. */ #ifndef VASNPRINTF # if WIDE_CHAR_VERSION # include "vasnwprintf.h" # else # include "vasnprintf.h" # endif #endif #include /* localeconv() */ #include /* snprintf(), sprintf() */ #include /* abort(), malloc(), realloc(), free() */ #include /* memcpy(), strlen() */ #include /* errno */ #include /* CHAR_BIT */ #include /* DBL_MAX_EXP, LDBL_MAX_EXP */ #if HAVE_NL_LANGINFO # include #endif #ifndef VASNPRINTF # if WIDE_CHAR_VERSION # include "wprintf-parse.h" # else # include "printf-parse.h" # endif #endif /* Checked size_t computations. */ #include "xsize.h" #include "verify.h" #if (NEED_PRINTF_DOUBLE || NEED_PRINTF_LONG_DOUBLE) && !defined IN_LIBINTL # include # include "float+.h" #endif #if (NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_DOUBLE) && !defined IN_LIBINTL # include # include "isnand-nolibm.h" #endif #if (NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_INFINITE_LONG_DOUBLE) && !defined IN_LIBINTL # include # include "isnanl-nolibm.h" # include "fpucw.h" #endif #if (NEED_PRINTF_DIRECTIVE_A || NEED_PRINTF_DOUBLE) && !defined IN_LIBINTL # include # include "isnand-nolibm.h" # include "printf-frexp.h" #endif #if (NEED_PRINTF_DIRECTIVE_A || NEED_PRINTF_LONG_DOUBLE) && !defined IN_LIBINTL # include # include "isnanl-nolibm.h" # include "printf-frexpl.h" # include "fpucw.h" #endif /* Default parameters. */ #ifndef VASNPRINTF # if WIDE_CHAR_VERSION # define VASNPRINTF vasnwprintf # define FCHAR_T wchar_t # define DCHAR_T wchar_t # define TCHAR_T wchar_t # define DCHAR_IS_TCHAR 1 # define DIRECTIVE wchar_t_directive # define DIRECTIVES wchar_t_directives # define PRINTF_PARSE wprintf_parse # define DCHAR_CPY wmemcpy # define DCHAR_SET wmemset # else # define VASNPRINTF vasnprintf # define FCHAR_T char # define DCHAR_T char # define TCHAR_T char # define DCHAR_IS_TCHAR 1 # define DIRECTIVE char_directive # define DIRECTIVES char_directives # define PRINTF_PARSE printf_parse # define DCHAR_CPY memcpy # define DCHAR_SET memset # endif #endif #if WIDE_CHAR_VERSION /* TCHAR_T is wchar_t. */ # define USE_SNPRINTF 1 # if HAVE_DECL__SNWPRINTF /* On Windows, the function swprintf() has a different signature than on Unix; we use the function _snwprintf() or - on mingw - snwprintf() instead. The mingw function snwprintf() has fewer bugs than the MSVCRT function _snwprintf(), so prefer that. */ # if defined __MINGW32__ # define SNPRINTF snwprintf # else # define SNPRINTF _snwprintf # endif # else /* Unix. */ # define SNPRINTF swprintf # endif #else /* TCHAR_T is char. */ /* Use snprintf if it exists under the name 'snprintf' or '_snprintf'. But don't use it on BeOS, since BeOS snprintf produces no output if the size argument is >= 0x3000000. Also don't use it on Linux libc5, since there snprintf with size = 1 writes any output without bounds, like sprintf. */ # if (HAVE_DECL__SNPRINTF || HAVE_SNPRINTF) && !defined __BEOS__ && !(__GNU_LIBRARY__ == 1) # define USE_SNPRINTF 1 # else # define USE_SNPRINTF 0 # endif # if HAVE_DECL__SNPRINTF /* Windows. The mingw function snprintf() has fewer bugs than the MSVCRT function _snprintf(), so prefer that. */ # if defined __MINGW32__ # define SNPRINTF snprintf /* Here we need to call the native snprintf, not rpl_snprintf. */ # undef snprintf # else # define SNPRINTF _snprintf # endif # else /* Unix. */ # define SNPRINTF snprintf /* Here we need to call the native snprintf, not rpl_snprintf. */ # undef snprintf # endif #endif /* Here we need to call the native sprintf, not rpl_sprintf. */ #undef sprintf /* GCC >= 4.0 with -Wall emits unjustified "... may be used uninitialized" warnings in this file. Use -Dlint to suppress them. */ #if defined GCC_LINT || defined lint # define IF_LINT(Code) Code #else # define IF_LINT(Code) /* empty */ #endif /* Avoid some warnings from "gcc -Wshadow". This file doesn't use the exp() and remainder() functions. */ #undef exp #define exp expo #undef remainder #define remainder rem #if (!USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99) && !WIDE_CHAR_VERSION # if (HAVE_STRNLEN && !defined _AIX) # define local_strnlen strnlen # else # ifndef local_strnlen_defined # define local_strnlen_defined 1 static size_t local_strnlen (const char *string, size_t maxlen) { const char *end = memchr (string, '\0', maxlen); return end ? (size_t) (end - string) : maxlen; } # endif # endif #endif #if (((!USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99) && WIDE_CHAR_VERSION) || ((!USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || (NEED_PRINTF_DIRECTIVE_LS && !defined IN_LIBINTL)) && !WIDE_CHAR_VERSION && DCHAR_IS_TCHAR)) && HAVE_WCHAR_T # if HAVE_WCSLEN # define local_wcslen wcslen # else /* Solaris 2.5.1 has wcslen() in a separate library libw.so. To avoid a dependency towards this library, here is a local substitute. Define this substitute only once, even if this file is included twice in the same compilation unit. */ # ifndef local_wcslen_defined # define local_wcslen_defined 1 static size_t local_wcslen (const wchar_t *s) { const wchar_t *ptr; for (ptr = s; *ptr != (wchar_t) 0; ptr++) ; return ptr - s; } # endif # endif #endif #if (!USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99) && HAVE_WCHAR_T && WIDE_CHAR_VERSION # if HAVE_WCSNLEN # define local_wcsnlen wcsnlen # else # ifndef local_wcsnlen_defined # define local_wcsnlen_defined 1 static size_t local_wcsnlen (const wchar_t *s, size_t maxlen) { const wchar_t *ptr; for (ptr = s; maxlen > 0 && *ptr != (wchar_t) 0; ptr++, maxlen--) ; return ptr - s; } # endif # endif #endif #if (NEED_PRINTF_DIRECTIVE_A || NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_INFINITE_LONG_DOUBLE || NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_DOUBLE) && !defined IN_LIBINTL /* Determine the decimal-point character according to the current locale. */ # ifndef decimal_point_char_defined # define decimal_point_char_defined 1 static char decimal_point_char (void) { const char *point; /* Determine it in a multithread-safe way. We know nl_langinfo is multithread-safe on glibc systems and Mac OS X systems, but is not required to be multithread-safe by POSIX. sprintf(), however, is multithread-safe. localeconv() is rarely multithread-safe. */ # if HAVE_NL_LANGINFO && (__GLIBC__ || defined __UCLIBC__ || (defined __APPLE__ && defined __MACH__)) point = nl_langinfo (RADIXCHAR); # elif 1 char pointbuf[5]; sprintf (pointbuf, "%#.0f", 1.0); point = &pointbuf[1]; # else point = localeconv () -> decimal_point; # endif /* The decimal point is always a single byte: either '.' or ','. */ return (point[0] != '\0' ? point[0] : '.'); } # endif #endif #if NEED_PRINTF_INFINITE_DOUBLE && !NEED_PRINTF_DOUBLE && !defined IN_LIBINTL /* Equivalent to !isfinite(x) || x == 0, but does not require libm. */ static int is_infinite_or_zero (double x) { return isnand (x) || x + x == x; } #endif #if NEED_PRINTF_INFINITE_LONG_DOUBLE && !NEED_PRINTF_LONG_DOUBLE && !defined IN_LIBINTL /* Equivalent to !isfinite(x) || x == 0, but does not require libm. */ static int is_infinite_or_zerol (long double x) { return isnanl (x) || x + x == x; } #endif #if (NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_DOUBLE) && !defined IN_LIBINTL /* Converting 'long double' to decimal without rare rounding bugs requires real bignums. We use the naming conventions of GNU gmp, but vastly simpler (and slower) algorithms. */ typedef unsigned int mp_limb_t; # define GMP_LIMB_BITS 32 verify (sizeof (mp_limb_t) * CHAR_BIT == GMP_LIMB_BITS); typedef unsigned long long mp_twolimb_t; # define GMP_TWOLIMB_BITS 64 verify (sizeof (mp_twolimb_t) * CHAR_BIT == GMP_TWOLIMB_BITS); /* Representation of a bignum >= 0. */ typedef struct { size_t nlimbs; mp_limb_t *limbs; /* Bits in little-endian order, allocated with malloc(). */ } mpn_t; /* Compute the product of two bignums >= 0. Return the allocated memory in case of success, NULL in case of memory allocation failure. */ static void * multiply (mpn_t src1, mpn_t src2, mpn_t *dest) { const mp_limb_t *p1; const mp_limb_t *p2; size_t len1; size_t len2; if (src1.nlimbs <= src2.nlimbs) { len1 = src1.nlimbs; p1 = src1.limbs; len2 = src2.nlimbs; p2 = src2.limbs; } else { len1 = src2.nlimbs; p1 = src2.limbs; len2 = src1.nlimbs; p2 = src1.limbs; } /* Now 0 <= len1 <= len2. */ if (len1 == 0) { /* src1 or src2 is zero. */ dest->nlimbs = 0; dest->limbs = (mp_limb_t *) malloc (1); } else { /* Here 1 <= len1 <= len2. */ size_t dlen; mp_limb_t *dp; size_t k, i, j; dlen = len1 + len2; dp = (mp_limb_t *) malloc (dlen * sizeof (mp_limb_t)); if (dp == NULL) return NULL; for (k = len2; k > 0; ) dp[--k] = 0; for (i = 0; i < len1; i++) { mp_limb_t digit1 = p1[i]; mp_twolimb_t carry = 0; for (j = 0; j < len2; j++) { mp_limb_t digit2 = p2[j]; carry += (mp_twolimb_t) digit1 * (mp_twolimb_t) digit2; carry += dp[i + j]; dp[i + j] = (mp_limb_t) carry; carry = carry >> GMP_LIMB_BITS; } dp[i + len2] = (mp_limb_t) carry; } /* Normalise. */ while (dlen > 0 && dp[dlen - 1] == 0) dlen--; dest->nlimbs = dlen; dest->limbs = dp; } return dest->limbs; } /* Compute the quotient of a bignum a >= 0 and a bignum b > 0. a is written as a = q * b + r with 0 <= r < b. q is the quotient, r the remainder. Finally, round-to-even is performed: If r > b/2 or if r = b/2 and q is odd, q is incremented. Return the allocated memory in case of success, NULL in case of memory allocation failure. */ static void * divide (mpn_t a, mpn_t b, mpn_t *q) { /* Algorithm: First normalise a and b: a=[a[m-1],...,a[0]], b=[b[n-1],...,b[0]] with m>=0 and n>0 (in base beta = 2^GMP_LIMB_BITS). If m=n=1, perform a single-precision division: r:=0, j:=m, while j>0 do {Here (q[m-1]*beta^(m-1)+...+q[j]*beta^j) * b[0] + r*beta^j = = a[m-1]*beta^(m-1)+...+a[j]*beta^j und 0<=r=n>1, perform a multiple-precision division: We have a/b < beta^(m-n+1). s:=intDsize-1-(highest bit in b[n-1]), 0<=s=beta/2. For j=m-n,...,0: {Here 0 <= r < b*beta^(j+1).} Compute q* : q* := floor((r[j+n]*beta+r[j+n-1])/b[n-1]). In case of overflow (q* >= beta) set q* := beta-1. Compute c2 := ((r[j+n]*beta+r[j+n-1]) - q* * b[n-1])*beta + r[j+n-2] and c3 := b[n-2] * q*. {We have 0 <= c2 < 2*beta^2, even 0 <= c2 < beta^2 if no overflow occurred. Furthermore 0 <= c3 < beta^2. If there was overflow and r[j+n]*beta+r[j+n-1] - q* * b[n-1] >= beta, i.e. c2 >= beta^2, the next test can be skipped.} While c3 > c2, {Here 0 <= c2 < c3 < beta^2} Put q* := q* - 1, c2 := c2 + b[n-1]*beta, c3 := c3 - b[n-2]. If q* > 0: Put r := r - b * q* * beta^j. In detail: [r[n+j],...,r[j]] := [r[n+j],...,r[j]] - q* * [b[n-1],...,b[0]]. hence: u:=0, for i:=0 to n-1 do u := u + q* * b[i], r[j+i]:=r[j+i]-(u mod beta) (+ beta, if carry), u:=u div beta (+ 1, if carry in subtraction) r[n+j]:=r[n+j]-u. {Since always u = (q* * [b[i-1],...,b[0]] div beta^i) + 1 < q* + 1 <= beta, the carry u does not overflow.} If a negative carry occurs, put q* := q* - 1 and [r[n+j],...,r[j]] := [r[n+j],...,r[j]] + [0,b[n-1],...,b[0]]. Set q[j] := q*. Normalise [q[m-n],..,q[0]]; this yields the quotient q. Shift [r[n-1],...,r[0]] right by s bits and normalise; this yields the rest r. The room for q[j] can be allocated at the memory location of r[n+j]. Finally, round-to-even: Shift r left by 1 bit. If r > b or if r = b and q[0] is odd, q := q+1. */ const mp_limb_t *a_ptr = a.limbs; size_t a_len = a.nlimbs; const mp_limb_t *b_ptr = b.limbs; size_t b_len = b.nlimbs; mp_limb_t *roomptr; mp_limb_t *tmp_roomptr = NULL; mp_limb_t *q_ptr; size_t q_len; mp_limb_t *r_ptr; size_t r_len; /* Allocate room for a_len+2 digits. (Need a_len+1 digits for the real division and 1 more digit for the final rounding of q.) */ roomptr = (mp_limb_t *) malloc ((a_len + 2) * sizeof (mp_limb_t)); if (roomptr == NULL) return NULL; /* Normalise a. */ while (a_len > 0 && a_ptr[a_len - 1] == 0) a_len--; /* Normalise b. */ for (;;) { if (b_len == 0) /* Division by zero. */ abort (); if (b_ptr[b_len - 1] == 0) b_len--; else break; } /* Here m = a_len >= 0 and n = b_len > 0. */ if (a_len < b_len) { /* m beta^(m-2) <= a/b < beta^m */ r_ptr = roomptr; q_ptr = roomptr + 1; { mp_limb_t den = b_ptr[0]; mp_limb_t remainder = 0; const mp_limb_t *sourceptr = a_ptr + a_len; mp_limb_t *destptr = q_ptr + a_len; size_t count; for (count = a_len; count > 0; count--) { mp_twolimb_t num = ((mp_twolimb_t) remainder << GMP_LIMB_BITS) | *--sourceptr; *--destptr = num / den; remainder = num % den; } /* Normalise and store r. */ if (remainder > 0) { r_ptr[0] = remainder; r_len = 1; } else r_len = 0; /* Normalise q. */ q_len = a_len; if (q_ptr[q_len - 1] == 0) q_len--; } } else { /* n>1: multiple precision division. beta^(m-1) <= a < beta^m, beta^(n-1) <= b < beta^n ==> beta^(m-n-1) <= a/b < beta^(m-n+1). */ /* Determine s. */ size_t s; { mp_limb_t msd = b_ptr[b_len - 1]; /* = b[n-1], > 0 */ /* Determine s = GMP_LIMB_BITS - integer_length (msd). Code copied from gnulib's integer_length.c. */ # if __GNUC__ > 3 || (__GNUC__ == 3 && __GNUC_MINOR__ >= 4) s = __builtin_clz (msd); # else # if defined DBL_EXPBIT0_WORD && defined DBL_EXPBIT0_BIT if (GMP_LIMB_BITS <= DBL_MANT_BIT) { /* Use 'double' operations. Assumes an IEEE 754 'double' implementation. */ # define DBL_EXP_MASK ((DBL_MAX_EXP - DBL_MIN_EXP) | 7) # define DBL_EXP_BIAS (DBL_EXP_MASK / 2 - 1) # define NWORDS \ ((sizeof (double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) union { double value; unsigned int word[NWORDS]; } m; /* Use a single integer to floating-point conversion. */ m.value = msd; s = GMP_LIMB_BITS - (((m.word[DBL_EXPBIT0_WORD] >> DBL_EXPBIT0_BIT) & DBL_EXP_MASK) - DBL_EXP_BIAS); } else # undef NWORDS # endif { s = 31; if (msd >= 0x10000) { msd = msd >> 16; s -= 16; } if (msd >= 0x100) { msd = msd >> 8; s -= 8; } if (msd >= 0x10) { msd = msd >> 4; s -= 4; } if (msd >= 0x4) { msd = msd >> 2; s -= 2; } if (msd >= 0x2) { msd = msd >> 1; s -= 1; } } # endif } /* 0 <= s < GMP_LIMB_BITS. Copy b, shifting it left by s bits. */ if (s > 0) { tmp_roomptr = (mp_limb_t *) malloc (b_len * sizeof (mp_limb_t)); if (tmp_roomptr == NULL) { free (roomptr); return NULL; } { const mp_limb_t *sourceptr = b_ptr; mp_limb_t *destptr = tmp_roomptr; mp_twolimb_t accu = 0; size_t count; for (count = b_len; count > 0; count--) { accu += (mp_twolimb_t) *sourceptr++ << s; *destptr++ = (mp_limb_t) accu; accu = accu >> GMP_LIMB_BITS; } /* accu must be zero, since that was how s was determined. */ if (accu != 0) abort (); } b_ptr = tmp_roomptr; } /* Copy a, shifting it left by s bits, yields r. Memory layout: At the beginning: r = roomptr[0..a_len], at the end: r = roomptr[0..b_len-1], q = roomptr[b_len..a_len] */ r_ptr = roomptr; if (s == 0) { memcpy (r_ptr, a_ptr, a_len * sizeof (mp_limb_t)); r_ptr[a_len] = 0; } else { const mp_limb_t *sourceptr = a_ptr; mp_limb_t *destptr = r_ptr; mp_twolimb_t accu = 0; size_t count; for (count = a_len; count > 0; count--) { accu += (mp_twolimb_t) *sourceptr++ << s; *destptr++ = (mp_limb_t) accu; accu = accu >> GMP_LIMB_BITS; } *destptr++ = (mp_limb_t) accu; } q_ptr = roomptr + b_len; q_len = a_len - b_len + 1; /* q will have m-n+1 limbs */ { size_t j = a_len - b_len; /* m-n */ mp_limb_t b_msd = b_ptr[b_len - 1]; /* b[n-1] */ mp_limb_t b_2msd = b_ptr[b_len - 2]; /* b[n-2] */ mp_twolimb_t b_msdd = /* b[n-1]*beta+b[n-2] */ ((mp_twolimb_t) b_msd << GMP_LIMB_BITS) | b_2msd; /* Division loop, traversed m-n+1 times. j counts down, b is unchanged, beta/2 <= b[n-1] < beta. */ for (;;) { mp_limb_t q_star; mp_limb_t c1; if (r_ptr[j + b_len] < b_msd) /* r[j+n] < b[n-1] ? */ { /* Divide r[j+n]*beta+r[j+n-1] by b[n-1], no overflow. */ mp_twolimb_t num = ((mp_twolimb_t) r_ptr[j + b_len] << GMP_LIMB_BITS) | r_ptr[j + b_len - 1]; q_star = num / b_msd; c1 = num % b_msd; } else { /* Overflow, hence r[j+n]*beta+r[j+n-1] >= beta*b[n-1]. */ q_star = (mp_limb_t)~(mp_limb_t)0; /* q* = beta-1 */ /* Test whether r[j+n]*beta+r[j+n-1] - (beta-1)*b[n-1] >= beta <==> r[j+n]*beta+r[j+n-1] + b[n-1] >= beta*b[n-1]+beta <==> b[n-1] < floor((r[j+n]*beta+r[j+n-1]+b[n-1])/beta) {<= beta !}. If yes, jump directly to the subtraction loop. (Otherwise, r[j+n]*beta+r[j+n-1] - (beta-1)*b[n-1] < beta <==> floor((r[j+n]*beta+r[j+n-1]+b[n-1])/beta) = b[n-1] ) */ if (r_ptr[j + b_len] > b_msd || (c1 = r_ptr[j + b_len - 1] + b_msd) < b_msd) /* r[j+n] >= b[n-1]+1 or r[j+n] = b[n-1] and the addition r[j+n-1]+b[n-1] gives a carry. */ goto subtract; } /* q_star = q*, c1 = (r[j+n]*beta+r[j+n-1]) - q* * b[n-1] (>=0, 0, decrease it by b[n-1]*beta+b[n-2]. Because of b[n-1]*beta+b[n-2] >= beta^2/2 this can happen only twice. */ if (c3 > c2) { q_star = q_star - 1; /* q* := q* - 1 */ if (c3 - c2 > b_msdd) q_star = q_star - 1; /* q* := q* - 1 */ } } if (q_star > 0) subtract: { /* Subtract r := r - b * q* * beta^j. */ mp_limb_t cr; { const mp_limb_t *sourceptr = b_ptr; mp_limb_t *destptr = r_ptr + j; mp_twolimb_t carry = 0; size_t count; for (count = b_len; count > 0; count--) { /* Here 0 <= carry <= q*. */ carry = carry + (mp_twolimb_t) q_star * (mp_twolimb_t) *sourceptr++ + (mp_limb_t) ~(*destptr); /* Here 0 <= carry <= beta*q* + beta-1. */ *destptr++ = ~(mp_limb_t) carry; carry = carry >> GMP_LIMB_BITS; /* <= q* */ } cr = (mp_limb_t) carry; } /* Subtract cr from r_ptr[j + b_len], then forget about r_ptr[j + b_len]. */ if (cr > r_ptr[j + b_len]) { /* Subtraction gave a carry. */ q_star = q_star - 1; /* q* := q* - 1 */ /* Add b back. */ { const mp_limb_t *sourceptr = b_ptr; mp_limb_t *destptr = r_ptr + j; mp_limb_t carry = 0; size_t count; for (count = b_len; count > 0; count--) { mp_limb_t source1 = *sourceptr++; mp_limb_t source2 = *destptr; *destptr++ = source1 + source2 + carry; carry = (carry ? source1 >= (mp_limb_t) ~source2 : source1 > (mp_limb_t) ~source2); } } /* Forget about the carry and about r[j+n]. */ } } /* q* is determined. Store it as q[j]. */ q_ptr[j] = q_star; if (j == 0) break; j--; } } r_len = b_len; /* Normalise q. */ if (q_ptr[q_len - 1] == 0) q_len--; # if 0 /* Not needed here, since we need r only to compare it with b/2, and b is shifted left by s bits. */ /* Shift r right by s bits. */ if (s > 0) { mp_limb_t ptr = r_ptr + r_len; mp_twolimb_t accu = 0; size_t count; for (count = r_len; count > 0; count--) { accu = (mp_twolimb_t) (mp_limb_t) accu << GMP_LIMB_BITS; accu += (mp_twolimb_t) *--ptr << (GMP_LIMB_BITS - s); *ptr = (mp_limb_t) (accu >> GMP_LIMB_BITS); } } # endif /* Normalise r. */ while (r_len > 0 && r_ptr[r_len - 1] == 0) r_len--; } /* Compare r << 1 with b. */ if (r_len > b_len) goto increment_q; { size_t i; for (i = b_len;;) { mp_limb_t r_i = (i <= r_len && i > 0 ? r_ptr[i - 1] >> (GMP_LIMB_BITS - 1) : 0) | (i < r_len ? r_ptr[i] << 1 : 0); mp_limb_t b_i = (i < b_len ? b_ptr[i] : 0); if (r_i > b_i) goto increment_q; if (r_i < b_i) goto keep_q; if (i == 0) break; i--; } } if (q_len > 0 && ((q_ptr[0] & 1) != 0)) /* q is odd. */ increment_q: { size_t i; for (i = 0; i < q_len; i++) if (++(q_ptr[i]) != 0) goto keep_q; q_ptr[q_len++] = 1; } keep_q: if (tmp_roomptr != NULL) free (tmp_roomptr); q->limbs = q_ptr; q->nlimbs = q_len; return roomptr; } /* Convert a bignum a >= 0, multiplied with 10^extra_zeroes, to decimal representation. Destroys the contents of a. Return the allocated memory - containing the decimal digits in low-to-high order, terminated with a NUL character - in case of success, NULL in case of memory allocation failure. */ static char * convert_to_decimal (mpn_t a, size_t extra_zeroes) { mp_limb_t *a_ptr = a.limbs; size_t a_len = a.nlimbs; /* 0.03345 is slightly larger than log(2)/(9*log(10)). */ size_t c_len = 9 * ((size_t)(a_len * (GMP_LIMB_BITS * 0.03345f)) + 1); char *c_ptr = (char *) malloc (xsum (c_len, extra_zeroes)); if (c_ptr != NULL) { char *d_ptr = c_ptr; for (; extra_zeroes > 0; extra_zeroes--) *d_ptr++ = '0'; while (a_len > 0) { /* Divide a by 10^9, in-place. */ mp_limb_t remainder = 0; mp_limb_t *ptr = a_ptr + a_len; size_t count; for (count = a_len; count > 0; count--) { mp_twolimb_t num = ((mp_twolimb_t) remainder << GMP_LIMB_BITS) | *--ptr; *ptr = num / 1000000000; remainder = num % 1000000000; } /* Store the remainder as 9 decimal digits. */ for (count = 9; count > 0; count--) { *d_ptr++ = '0' + (remainder % 10); remainder = remainder / 10; } /* Normalize a. */ if (a_ptr[a_len - 1] == 0) a_len--; } /* Remove leading zeroes. */ while (d_ptr > c_ptr && d_ptr[-1] == '0') d_ptr--; /* But keep at least one zero. */ if (d_ptr == c_ptr) *d_ptr++ = '0'; /* Terminate the string. */ *d_ptr = '\0'; } return c_ptr; } # if NEED_PRINTF_LONG_DOUBLE /* Assuming x is finite and >= 0: write x as x = 2^e * m, where m is a bignum. Return the allocated memory in case of success, NULL in case of memory allocation failure. */ static void * decode_long_double (long double x, int *ep, mpn_t *mp) { mpn_t m; int exp; long double y; size_t i; /* Allocate memory for result. */ m.nlimbs = (LDBL_MANT_BIT + GMP_LIMB_BITS - 1) / GMP_LIMB_BITS; m.limbs = (mp_limb_t *) malloc (m.nlimbs * sizeof (mp_limb_t)); if (m.limbs == NULL) return NULL; /* Split into exponential part and mantissa. */ y = frexpl (x, &exp); if (!(y >= 0.0L && y < 1.0L)) abort (); /* x = 2^exp * y = 2^(exp - LDBL_MANT_BIT) * (y * 2^LDBL_MANT_BIT), and the latter is an integer. */ /* Convert the mantissa (y * 2^LDBL_MANT_BIT) to a sequence of limbs. I'm not sure whether it's safe to cast a 'long double' value between 2^31 and 2^32 to 'unsigned int', therefore play safe and cast only 'long double' values between 0 and 2^16 (to 'unsigned int' or 'int', doesn't matter). */ # if (LDBL_MANT_BIT % GMP_LIMB_BITS) != 0 # if (LDBL_MANT_BIT % GMP_LIMB_BITS) > GMP_LIMB_BITS / 2 { mp_limb_t hi, lo; y *= (mp_limb_t) 1 << (LDBL_MANT_BIT % (GMP_LIMB_BITS / 2)); hi = (int) y; y -= hi; if (!(y >= 0.0L && y < 1.0L)) abort (); y *= (mp_limb_t) 1 << (GMP_LIMB_BITS / 2); lo = (int) y; y -= lo; if (!(y >= 0.0L && y < 1.0L)) abort (); m.limbs[LDBL_MANT_BIT / GMP_LIMB_BITS] = (hi << (GMP_LIMB_BITS / 2)) | lo; } # else { mp_limb_t d; y *= (mp_limb_t) 1 << (LDBL_MANT_BIT % GMP_LIMB_BITS); d = (int) y; y -= d; if (!(y >= 0.0L && y < 1.0L)) abort (); m.limbs[LDBL_MANT_BIT / GMP_LIMB_BITS] = d; } # endif # endif for (i = LDBL_MANT_BIT / GMP_LIMB_BITS; i > 0; ) { mp_limb_t hi, lo; y *= (mp_limb_t) 1 << (GMP_LIMB_BITS / 2); hi = (int) y; y -= hi; if (!(y >= 0.0L && y < 1.0L)) abort (); y *= (mp_limb_t) 1 << (GMP_LIMB_BITS / 2); lo = (int) y; y -= lo; if (!(y >= 0.0L && y < 1.0L)) abort (); m.limbs[--i] = (hi << (GMP_LIMB_BITS / 2)) | lo; } # if 0 /* On FreeBSD 6.1/x86, 'long double' numbers sometimes have excess precision. */ if (!(y == 0.0L)) abort (); # endif /* Normalise. */ while (m.nlimbs > 0 && m.limbs[m.nlimbs - 1] == 0) m.nlimbs--; *mp = m; *ep = exp - LDBL_MANT_BIT; return m.limbs; } # endif # if NEED_PRINTF_DOUBLE /* Assuming x is finite and >= 0: write x as x = 2^e * m, where m is a bignum. Return the allocated memory in case of success, NULL in case of memory allocation failure. */ static void * decode_double (double x, int *ep, mpn_t *mp) { mpn_t m; int exp; double y; size_t i; /* Allocate memory for result. */ m.nlimbs = (DBL_MANT_BIT + GMP_LIMB_BITS - 1) / GMP_LIMB_BITS; m.limbs = (mp_limb_t *) malloc (m.nlimbs * sizeof (mp_limb_t)); if (m.limbs == NULL) return NULL; /* Split into exponential part and mantissa. */ y = frexp (x, &exp); if (!(y >= 0.0 && y < 1.0)) abort (); /* x = 2^exp * y = 2^(exp - DBL_MANT_BIT) * (y * 2^DBL_MANT_BIT), and the latter is an integer. */ /* Convert the mantissa (y * 2^DBL_MANT_BIT) to a sequence of limbs. I'm not sure whether it's safe to cast a 'double' value between 2^31 and 2^32 to 'unsigned int', therefore play safe and cast only 'double' values between 0 and 2^16 (to 'unsigned int' or 'int', doesn't matter). */ # if (DBL_MANT_BIT % GMP_LIMB_BITS) != 0 # if (DBL_MANT_BIT % GMP_LIMB_BITS) > GMP_LIMB_BITS / 2 { mp_limb_t hi, lo; y *= (mp_limb_t) 1 << (DBL_MANT_BIT % (GMP_LIMB_BITS / 2)); hi = (int) y; y -= hi; if (!(y >= 0.0 && y < 1.0)) abort (); y *= (mp_limb_t) 1 << (GMP_LIMB_BITS / 2); lo = (int) y; y -= lo; if (!(y >= 0.0 && y < 1.0)) abort (); m.limbs[DBL_MANT_BIT / GMP_LIMB_BITS] = (hi << (GMP_LIMB_BITS / 2)) | lo; } # else { mp_limb_t d; y *= (mp_limb_t) 1 << (DBL_MANT_BIT % GMP_LIMB_BITS); d = (int) y; y -= d; if (!(y >= 0.0 && y < 1.0)) abort (); m.limbs[DBL_MANT_BIT / GMP_LIMB_BITS] = d; } # endif # endif for (i = DBL_MANT_BIT / GMP_LIMB_BITS; i > 0; ) { mp_limb_t hi, lo; y *= (mp_limb_t) 1 << (GMP_LIMB_BITS / 2); hi = (int) y; y -= hi; if (!(y >= 0.0 && y < 1.0)) abort (); y *= (mp_limb_t) 1 << (GMP_LIMB_BITS / 2); lo = (int) y; y -= lo; if (!(y >= 0.0 && y < 1.0)) abort (); m.limbs[--i] = (hi << (GMP_LIMB_BITS / 2)) | lo; } if (!(y == 0.0)) abort (); /* Normalise. */ while (m.nlimbs > 0 && m.limbs[m.nlimbs - 1] == 0) m.nlimbs--; *mp = m; *ep = exp - DBL_MANT_BIT; return m.limbs; } # endif /* Assuming x = 2^e * m is finite and >= 0, and n is an integer: Returns the decimal representation of round (x * 10^n). Return the allocated memory - containing the decimal digits in low-to-high order, terminated with a NUL character - in case of success, NULL in case of memory allocation failure. */ static char * scale10_round_decimal_decoded (int e, mpn_t m, void *memory, int n) { int s; size_t extra_zeroes; unsigned int abs_n; unsigned int abs_s; mp_limb_t *pow5_ptr; size_t pow5_len; unsigned int s_limbs; unsigned int s_bits; mpn_t pow5; mpn_t z; void *z_memory; char *digits; if (memory == NULL) return NULL; /* x = 2^e * m, hence y = round (2^e * 10^n * m) = round (2^(e+n) * 5^n * m) = round (2^s * 5^n * m). */ s = e + n; extra_zeroes = 0; /* Factor out a common power of 10 if possible. */ if (s > 0 && n > 0) { extra_zeroes = (s < n ? s : n); s -= extra_zeroes; n -= extra_zeroes; } /* Here y = round (2^s * 5^n * m) * 10^extra_zeroes. Before converting to decimal, we need to compute z = round (2^s * 5^n * m). */ /* Compute 5^|n|, possibly shifted by |s| bits if n and s have the same sign. 2.322 is slightly larger than log(5)/log(2). */ abs_n = (n >= 0 ? n : -n); abs_s = (s >= 0 ? s : -s); pow5_ptr = (mp_limb_t *) malloc (((int)(abs_n * (2.322f / GMP_LIMB_BITS)) + 1 + abs_s / GMP_LIMB_BITS + 1) * sizeof (mp_limb_t)); if (pow5_ptr == NULL) { free (memory); return NULL; } /* Initialize with 1. */ pow5_ptr[0] = 1; pow5_len = 1; /* Multiply with 5^|n|. */ if (abs_n > 0) { static mp_limb_t const small_pow5[13 + 1] = { 1, 5, 25, 125, 625, 3125, 15625, 78125, 390625, 1953125, 9765625, 48828125, 244140625, 1220703125 }; unsigned int n13; for (n13 = 0; n13 <= abs_n; n13 += 13) { mp_limb_t digit1 = small_pow5[n13 + 13 <= abs_n ? 13 : abs_n - n13]; size_t j; mp_twolimb_t carry = 0; for (j = 0; j < pow5_len; j++) { mp_limb_t digit2 = pow5_ptr[j]; carry += (mp_twolimb_t) digit1 * (mp_twolimb_t) digit2; pow5_ptr[j] = (mp_limb_t) carry; carry = carry >> GMP_LIMB_BITS; } if (carry > 0) pow5_ptr[pow5_len++] = (mp_limb_t) carry; } } s_limbs = abs_s / GMP_LIMB_BITS; s_bits = abs_s % GMP_LIMB_BITS; if (n >= 0 ? s >= 0 : s <= 0) { /* Multiply with 2^|s|. */ if (s_bits > 0) { mp_limb_t *ptr = pow5_ptr; mp_twolimb_t accu = 0; size_t count; for (count = pow5_len; count > 0; count--) { accu += (mp_twolimb_t) *ptr << s_bits; *ptr++ = (mp_limb_t) accu; accu = accu >> GMP_LIMB_BITS; } if (accu > 0) { *ptr = (mp_limb_t) accu; pow5_len++; } } if (s_limbs > 0) { size_t count; for (count = pow5_len; count > 0;) { count--; pow5_ptr[s_limbs + count] = pow5_ptr[count]; } for (count = s_limbs; count > 0;) { count--; pow5_ptr[count] = 0; } pow5_len += s_limbs; } pow5.limbs = pow5_ptr; pow5.nlimbs = pow5_len; if (n >= 0) { /* Multiply m with pow5. No division needed. */ z_memory = multiply (m, pow5, &z); } else { /* Divide m by pow5 and round. */ z_memory = divide (m, pow5, &z); } } else { pow5.limbs = pow5_ptr; pow5.nlimbs = pow5_len; if (n >= 0) { /* n >= 0, s < 0. Multiply m with pow5, then divide by 2^|s|. */ mpn_t numerator; mpn_t denominator; void *tmp_memory; tmp_memory = multiply (m, pow5, &numerator); if (tmp_memory == NULL) { free (pow5_ptr); free (memory); return NULL; } /* Construct 2^|s|. */ { mp_limb_t *ptr = pow5_ptr + pow5_len; size_t i; for (i = 0; i < s_limbs; i++) ptr[i] = 0; ptr[s_limbs] = (mp_limb_t) 1 << s_bits; denominator.limbs = ptr; denominator.nlimbs = s_limbs + 1; } z_memory = divide (numerator, denominator, &z); free (tmp_memory); } else { /* n < 0, s > 0. Multiply m with 2^s, then divide by pow5. */ mpn_t numerator; mp_limb_t *num_ptr; num_ptr = (mp_limb_t *) malloc ((m.nlimbs + s_limbs + 1) * sizeof (mp_limb_t)); if (num_ptr == NULL) { free (pow5_ptr); free (memory); return NULL; } { mp_limb_t *destptr = num_ptr; { size_t i; for (i = 0; i < s_limbs; i++) *destptr++ = 0; } if (s_bits > 0) { const mp_limb_t *sourceptr = m.limbs; mp_twolimb_t accu = 0; size_t count; for (count = m.nlimbs; count > 0; count--) { accu += (mp_twolimb_t) *sourceptr++ << s_bits; *destptr++ = (mp_limb_t) accu; accu = accu >> GMP_LIMB_BITS; } if (accu > 0) *destptr++ = (mp_limb_t) accu; } else { const mp_limb_t *sourceptr = m.limbs; size_t count; for (count = m.nlimbs; count > 0; count--) *destptr++ = *sourceptr++; } numerator.limbs = num_ptr; numerator.nlimbs = destptr - num_ptr; } z_memory = divide (numerator, pow5, &z); free (num_ptr); } } free (pow5_ptr); free (memory); /* Here y = round (x * 10^n) = z * 10^extra_zeroes. */ if (z_memory == NULL) return NULL; digits = convert_to_decimal (z, extra_zeroes); free (z_memory); return digits; } # if NEED_PRINTF_LONG_DOUBLE /* Assuming x is finite and >= 0, and n is an integer: Returns the decimal representation of round (x * 10^n). Return the allocated memory - containing the decimal digits in low-to-high order, terminated with a NUL character - in case of success, NULL in case of memory allocation failure. */ static char * scale10_round_decimal_long_double (long double x, int n) { int e IF_LINT(= 0); mpn_t m; void *memory = decode_long_double (x, &e, &m); return scale10_round_decimal_decoded (e, m, memory, n); } # endif # if NEED_PRINTF_DOUBLE /* Assuming x is finite and >= 0, and n is an integer: Returns the decimal representation of round (x * 10^n). Return the allocated memory - containing the decimal digits in low-to-high order, terminated with a NUL character - in case of success, NULL in case of memory allocation failure. */ static char * scale10_round_decimal_double (double x, int n) { int e IF_LINT(= 0); mpn_t m; void *memory = decode_double (x, &e, &m); return scale10_round_decimal_decoded (e, m, memory, n); } # endif # if NEED_PRINTF_LONG_DOUBLE /* Assuming x is finite and > 0: Return an approximation for n with 10^n <= x < 10^(n+1). The approximation is usually the right n, but may be off by 1 sometimes. */ static int floorlog10l (long double x) { int exp; long double y; double z; double l; /* Split into exponential part and mantissa. */ y = frexpl (x, &exp); if (!(y >= 0.0L && y < 1.0L)) abort (); if (y == 0.0L) return INT_MIN; if (y < 0.5L) { while (y < (1.0L / (1 << (GMP_LIMB_BITS / 2)) / (1 << (GMP_LIMB_BITS / 2)))) { y *= 1.0L * (1 << (GMP_LIMB_BITS / 2)) * (1 << (GMP_LIMB_BITS / 2)); exp -= GMP_LIMB_BITS; } if (y < (1.0L / (1 << 16))) { y *= 1.0L * (1 << 16); exp -= 16; } if (y < (1.0L / (1 << 8))) { y *= 1.0L * (1 << 8); exp -= 8; } if (y < (1.0L / (1 << 4))) { y *= 1.0L * (1 << 4); exp -= 4; } if (y < (1.0L / (1 << 2))) { y *= 1.0L * (1 << 2); exp -= 2; } if (y < (1.0L / (1 << 1))) { y *= 1.0L * (1 << 1); exp -= 1; } } if (!(y >= 0.5L && y < 1.0L)) abort (); /* Compute an approximation for l = log2(x) = exp + log2(y). */ l = exp; z = y; if (z < 0.70710678118654752444) { z *= 1.4142135623730950488; l -= 0.5; } if (z < 0.8408964152537145431) { z *= 1.1892071150027210667; l -= 0.25; } if (z < 0.91700404320467123175) { z *= 1.0905077326652576592; l -= 0.125; } if (z < 0.9576032806985736469) { z *= 1.0442737824274138403; l -= 0.0625; } /* Now 0.95 <= z <= 1.01. */ z = 1 - z; /* log2(1-z) = 1/log(2) * (- z - z^2/2 - z^3/3 - z^4/4 - ...) Four terms are enough to get an approximation with error < 10^-7. */ l -= 1.4426950408889634074 * z * (1.0 + z * (0.5 + z * ((1.0 / 3) + z * 0.25))); /* Finally multiply with log(2)/log(10), yields an approximation for log10(x). */ l *= 0.30102999566398119523; /* Round down to the next integer. */ return (int) l + (l < 0 ? -1 : 0); } # endif # if NEED_PRINTF_DOUBLE /* Assuming x is finite and > 0: Return an approximation for n with 10^n <= x < 10^(n+1). The approximation is usually the right n, but may be off by 1 sometimes. */ static int floorlog10 (double x) { int exp; double y; double z; double l; /* Split into exponential part and mantissa. */ y = frexp (x, &exp); if (!(y >= 0.0 && y < 1.0)) abort (); if (y == 0.0) return INT_MIN; if (y < 0.5) { while (y < (1.0 / (1 << (GMP_LIMB_BITS / 2)) / (1 << (GMP_LIMB_BITS / 2)))) { y *= 1.0 * (1 << (GMP_LIMB_BITS / 2)) * (1 << (GMP_LIMB_BITS / 2)); exp -= GMP_LIMB_BITS; } if (y < (1.0 / (1 << 16))) { y *= 1.0 * (1 << 16); exp -= 16; } if (y < (1.0 / (1 << 8))) { y *= 1.0 * (1 << 8); exp -= 8; } if (y < (1.0 / (1 << 4))) { y *= 1.0 * (1 << 4); exp -= 4; } if (y < (1.0 / (1 << 2))) { y *= 1.0 * (1 << 2); exp -= 2; } if (y < (1.0 / (1 << 1))) { y *= 1.0 * (1 << 1); exp -= 1; } } if (!(y >= 0.5 && y < 1.0)) abort (); /* Compute an approximation for l = log2(x) = exp + log2(y). */ l = exp; z = y; if (z < 0.70710678118654752444) { z *= 1.4142135623730950488; l -= 0.5; } if (z < 0.8408964152537145431) { z *= 1.1892071150027210667; l -= 0.25; } if (z < 0.91700404320467123175) { z *= 1.0905077326652576592; l -= 0.125; } if (z < 0.9576032806985736469) { z *= 1.0442737824274138403; l -= 0.0625; } /* Now 0.95 <= z <= 1.01. */ z = 1 - z; /* log2(1-z) = 1/log(2) * (- z - z^2/2 - z^3/3 - z^4/4 - ...) Four terms are enough to get an approximation with error < 10^-7. */ l -= 1.4426950408889634074 * z * (1.0 + z * (0.5 + z * ((1.0 / 3) + z * 0.25))); /* Finally multiply with log(2)/log(10), yields an approximation for log10(x). */ l *= 0.30102999566398119523; /* Round down to the next integer. */ return (int) l + (l < 0 ? -1 : 0); } # endif /* Tests whether a string of digits consists of exactly PRECISION zeroes and a single '1' digit. */ static int is_borderline (const char *digits, size_t precision) { for (; precision > 0; precision--, digits++) if (*digits != '0') return 0; if (*digits != '1') return 0; digits++; return *digits == '\0'; } #endif #if !USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 /* Use a different function name, to make it possible that the 'wchar_t' parametrization and the 'char' parametrization get compiled in the same translation unit. */ # if WIDE_CHAR_VERSION # define MAX_ROOM_NEEDED wmax_room_needed # else # define MAX_ROOM_NEEDED max_room_needed # endif /* Returns the number of TCHAR_T units needed as temporary space for the result of sprintf or SNPRINTF of a single conversion directive. */ static size_t MAX_ROOM_NEEDED (const arguments *ap, size_t arg_index, FCHAR_T conversion, arg_type type, int flags, size_t width, int has_precision, size_t precision, int pad_ourselves) { size_t tmp_length; switch (conversion) { case 'd': case 'i': case 'u': # if HAVE_LONG_LONG_INT if (type == TYPE_LONGLONGINT || type == TYPE_ULONGLONGINT) tmp_length = (unsigned int) (sizeof (unsigned long long) * CHAR_BIT * 0.30103 /* binary -> decimal */ ) + 1; /* turn floor into ceil */ else # endif if (type == TYPE_LONGINT || type == TYPE_ULONGINT) tmp_length = (unsigned int) (sizeof (unsigned long) * CHAR_BIT * 0.30103 /* binary -> decimal */ ) + 1; /* turn floor into ceil */ else tmp_length = (unsigned int) (sizeof (unsigned int) * CHAR_BIT * 0.30103 /* binary -> decimal */ ) + 1; /* turn floor into ceil */ if (tmp_length < precision) tmp_length = precision; /* Multiply by 2, as an estimate for FLAG_GROUP. */ tmp_length = xsum (tmp_length, tmp_length); /* Add 1, to account for a leading sign. */ tmp_length = xsum (tmp_length, 1); break; case 'o': # if HAVE_LONG_LONG_INT if (type == TYPE_LONGLONGINT || type == TYPE_ULONGLONGINT) tmp_length = (unsigned int) (sizeof (unsigned long long) * CHAR_BIT * 0.333334 /* binary -> octal */ ) + 1; /* turn floor into ceil */ else # endif if (type == TYPE_LONGINT || type == TYPE_ULONGINT) tmp_length = (unsigned int) (sizeof (unsigned long) * CHAR_BIT * 0.333334 /* binary -> octal */ ) + 1; /* turn floor into ceil */ else tmp_length = (unsigned int) (sizeof (unsigned int) * CHAR_BIT * 0.333334 /* binary -> octal */ ) + 1; /* turn floor into ceil */ if (tmp_length < precision) tmp_length = precision; /* Add 1, to account for a leading sign. */ tmp_length = xsum (tmp_length, 1); break; case 'x': case 'X': # if HAVE_LONG_LONG_INT if (type == TYPE_LONGLONGINT || type == TYPE_ULONGLONGINT) tmp_length = (unsigned int) (sizeof (unsigned long long) * CHAR_BIT * 0.25 /* binary -> hexadecimal */ ) + 1; /* turn floor into ceil */ else # endif if (type == TYPE_LONGINT || type == TYPE_ULONGINT) tmp_length = (unsigned int) (sizeof (unsigned long) * CHAR_BIT * 0.25 /* binary -> hexadecimal */ ) + 1; /* turn floor into ceil */ else tmp_length = (unsigned int) (sizeof (unsigned int) * CHAR_BIT * 0.25 /* binary -> hexadecimal */ ) + 1; /* turn floor into ceil */ if (tmp_length < precision) tmp_length = precision; /* Add 2, to account for a leading sign or alternate form. */ tmp_length = xsum (tmp_length, 2); break; case 'f': case 'F': if (type == TYPE_LONGDOUBLE) tmp_length = (unsigned int) (LDBL_MAX_EXP * 0.30103 /* binary -> decimal */ * 2 /* estimate for FLAG_GROUP */ ) + 1 /* turn floor into ceil */ + 10; /* sign, decimal point etc. */ else tmp_length = (unsigned int) (DBL_MAX_EXP * 0.30103 /* binary -> decimal */ * 2 /* estimate for FLAG_GROUP */ ) + 1 /* turn floor into ceil */ + 10; /* sign, decimal point etc. */ tmp_length = xsum (tmp_length, precision); break; case 'e': case 'E': case 'g': case 'G': tmp_length = 12; /* sign, decimal point, exponent etc. */ tmp_length = xsum (tmp_length, precision); break; case 'a': case 'A': if (type == TYPE_LONGDOUBLE) tmp_length = (unsigned int) (LDBL_DIG * 0.831 /* decimal -> hexadecimal */ ) + 1; /* turn floor into ceil */ else tmp_length = (unsigned int) (DBL_DIG * 0.831 /* decimal -> hexadecimal */ ) + 1; /* turn floor into ceil */ if (tmp_length < precision) tmp_length = precision; /* Account for sign, decimal point etc. */ tmp_length = xsum (tmp_length, 12); break; case 'c': # if HAVE_WINT_T && !WIDE_CHAR_VERSION if (type == TYPE_WIDE_CHAR) tmp_length = MB_CUR_MAX; else # endif tmp_length = 1; break; case 's': # if HAVE_WCHAR_T if (type == TYPE_WIDE_STRING) { # if WIDE_CHAR_VERSION /* ISO C says about %ls in fwprintf: "If the precision is not specified or is greater than the size of the array, the array shall contain a null wide character." So if there is a precision, we must not use wcslen. */ const wchar_t *arg = ap->arg[arg_index].a.a_wide_string; if (has_precision) tmp_length = local_wcsnlen (arg, precision); else tmp_length = local_wcslen (arg); # else /* ISO C says about %ls in fprintf: "If a precision is specified, no more than that many bytes are written (including shift sequences, if any), and the array shall contain a null wide character if, to equal the multibyte character sequence length given by the precision, the function would need to access a wide character one past the end of the array." So if there is a precision, we must not use wcslen. */ /* This case has already been handled separately in VASNPRINTF. */ abort (); # endif } else # endif { # if WIDE_CHAR_VERSION /* ISO C says about %s in fwprintf: "If the precision is not specified or is greater than the size of the converted array, the converted array shall contain a null wide character." So if there is a precision, we must not use strlen. */ /* This case has already been handled separately in VASNPRINTF. */ abort (); # else /* ISO C says about %s in fprintf: "If the precision is not specified or greater than the size of the array, the array shall contain a null character." So if there is a precision, we must not use strlen. */ const char *arg = ap->arg[arg_index].a.a_string; if (has_precision) tmp_length = local_strnlen (arg, precision); else tmp_length = strlen (arg); # endif } break; case 'p': tmp_length = (unsigned int) (sizeof (void *) * CHAR_BIT * 0.25 /* binary -> hexadecimal */ ) + 1 /* turn floor into ceil */ + 2; /* account for leading 0x */ break; default: abort (); } if (!pad_ourselves) { # if ENABLE_UNISTDIO /* Padding considers the number of characters, therefore the number of elements after padding may be > max (tmp_length, width) but is certainly <= tmp_length + width. */ tmp_length = xsum (tmp_length, width); # else /* Padding considers the number of elements, says POSIX. */ if (tmp_length < width) tmp_length = width; # endif } tmp_length = xsum (tmp_length, 1); /* account for trailing NUL */ return tmp_length; } #endif DCHAR_T * VASNPRINTF (DCHAR_T *resultbuf, size_t *lengthp, const FCHAR_T *format, va_list args) { DIRECTIVES d; arguments a; if (PRINTF_PARSE (format, &d, &a) < 0) /* errno is already set. */ return NULL; #define CLEANUP() \ if (d.dir != d.direct_alloc_dir) \ free (d.dir); \ if (a.arg != a.direct_alloc_arg) \ free (a.arg); if (PRINTF_FETCHARGS (args, &a) < 0) { CLEANUP (); errno = EINVAL; return NULL; } { size_t buf_neededlength; TCHAR_T *buf; TCHAR_T *buf_malloced; const FCHAR_T *cp; size_t i; DIRECTIVE *dp; /* Output string accumulator. */ DCHAR_T *result; size_t allocated; size_t length; /* Allocate a small buffer that will hold a directive passed to sprintf or snprintf. */ buf_neededlength = xsum4 (7, d.max_width_length, d.max_precision_length, 6); #if HAVE_ALLOCA if (buf_neededlength < 4000 / sizeof (TCHAR_T)) { buf = (TCHAR_T *) alloca (buf_neededlength * sizeof (TCHAR_T)); buf_malloced = NULL; } else #endif { size_t buf_memsize = xtimes (buf_neededlength, sizeof (TCHAR_T)); if (size_overflow_p (buf_memsize)) goto out_of_memory_1; buf = (TCHAR_T *) malloc (buf_memsize); if (buf == NULL) goto out_of_memory_1; buf_malloced = buf; } if (resultbuf != NULL) { result = resultbuf; allocated = *lengthp; } else { result = NULL; allocated = 0; } length = 0; /* Invariants: result is either == resultbuf or == NULL or malloc-allocated. If length > 0, then result != NULL. */ /* Ensures that allocated >= needed. Aborts through a jump to out_of_memory if needed is SIZE_MAX or otherwise too big. */ #define ENSURE_ALLOCATION(needed) \ if ((needed) > allocated) \ { \ size_t memory_size; \ DCHAR_T *memory; \ \ allocated = (allocated > 0 ? xtimes (allocated, 2) : 12); \ if ((needed) > allocated) \ allocated = (needed); \ memory_size = xtimes (allocated, sizeof (DCHAR_T)); \ if (size_overflow_p (memory_size)) \ goto out_of_memory; \ if (result == resultbuf || result == NULL) \ memory = (DCHAR_T *) malloc (memory_size); \ else \ memory = (DCHAR_T *) realloc (result, memory_size); \ if (memory == NULL) \ goto out_of_memory; \ if (result == resultbuf && length > 0) \ DCHAR_CPY (memory, result, length); \ result = memory; \ } for (cp = format, i = 0, dp = &d.dir[0]; ; cp = dp->dir_end, i++, dp++) { if (cp != dp->dir_start) { size_t n = dp->dir_start - cp; size_t augmented_length = xsum (length, n); ENSURE_ALLOCATION (augmented_length); /* This copies a piece of FCHAR_T[] into a DCHAR_T[]. Here we need that the format string contains only ASCII characters if FCHAR_T and DCHAR_T are not the same type. */ if (sizeof (FCHAR_T) == sizeof (DCHAR_T)) { DCHAR_CPY (result + length, (const DCHAR_T *) cp, n); length = augmented_length; } else { do result[length++] = *cp++; while (--n > 0); } } if (i == d.count) break; /* Execute a single directive. */ if (dp->conversion == '%') { size_t augmented_length; if (!(dp->arg_index == ARG_NONE)) abort (); augmented_length = xsum (length, 1); ENSURE_ALLOCATION (augmented_length); result[length] = '%'; length = augmented_length; } else { if (!(dp->arg_index != ARG_NONE)) abort (); if (dp->conversion == 'n') { switch (a.arg[dp->arg_index].type) { case TYPE_COUNT_SCHAR_POINTER: *a.arg[dp->arg_index].a.a_count_schar_pointer = length; break; case TYPE_COUNT_SHORT_POINTER: *a.arg[dp->arg_index].a.a_count_short_pointer = length; break; case TYPE_COUNT_INT_POINTER: *a.arg[dp->arg_index].a.a_count_int_pointer = length; break; case TYPE_COUNT_LONGINT_POINTER: *a.arg[dp->arg_index].a.a_count_longint_pointer = length; break; #if HAVE_LONG_LONG_INT case TYPE_COUNT_LONGLONGINT_POINTER: *a.arg[dp->arg_index].a.a_count_longlongint_pointer = length; break; #endif default: abort (); } } #if ENABLE_UNISTDIO /* The unistdio extensions. */ else if (dp->conversion == 'U') { arg_type type = a.arg[dp->arg_index].type; int flags = dp->flags; int has_width; size_t width; int has_precision; size_t precision; has_width = 0; width = 0; if (dp->width_start != dp->width_end) { if (dp->width_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->width_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->width_arg_index].a.a_int; width = arg; if (arg < 0) { /* "A negative field width is taken as a '-' flag followed by a positive field width." */ flags |= FLAG_LEFT; width = -width; } } else { const FCHAR_T *digitp = dp->width_start; do width = xsum (xtimes (width, 10), *digitp++ - '0'); while (digitp != dp->width_end); } has_width = 1; } has_precision = 0; precision = 0; if (dp->precision_start != dp->precision_end) { if (dp->precision_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->precision_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->precision_arg_index].a.a_int; /* "A negative precision is taken as if the precision were omitted." */ if (arg >= 0) { precision = arg; has_precision = 1; } } else { const FCHAR_T *digitp = dp->precision_start + 1; precision = 0; while (digitp != dp->precision_end) precision = xsum (xtimes (precision, 10), *digitp++ - '0'); has_precision = 1; } } switch (type) { case TYPE_U8_STRING: { const uint8_t *arg = a.arg[dp->arg_index].a.a_u8_string; const uint8_t *arg_end; size_t characters; if (has_precision) { /* Use only PRECISION characters, from the left. */ arg_end = arg; characters = 0; for (; precision > 0; precision--) { int count = u8_strmblen (arg_end); if (count == 0) break; if (count < 0) { if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else if (has_width) { /* Use the entire string, and count the number of characters. */ arg_end = arg; characters = 0; for (;;) { int count = u8_strmblen (arg_end); if (count == 0) break; if (count < 0) { if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else { /* Use the entire string. */ arg_end = arg + u8_strlen (arg); /* The number of characters doesn't matter. */ characters = 0; } if (characters < width && !(dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } # if DCHAR_IS_UINT8_T { size_t n = arg_end - arg; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_CPY (result + length, arg, n); length += n; } # else { /* Convert. */ DCHAR_T *converted = result + length; size_t converted_len = allocated - length; # if DCHAR_IS_TCHAR /* Convert from UTF-8 to locale encoding. */ converted = u8_conv_to_encoding (locale_charset (), iconveh_question_mark, arg, arg_end - arg, NULL, converted, &converted_len); # else /* Convert from UTF-8 to UTF-16/UTF-32. */ converted = U8_TO_DCHAR (arg, arg_end - arg, converted, &converted_len); # endif if (converted == NULL) { int saved_errno = errno; if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = saved_errno; return NULL; } if (converted != result + length) { ENSURE_ALLOCATION (xsum (length, converted_len)); DCHAR_CPY (result + length, converted, converted_len); free (converted); } length += converted_len; } # endif if (characters < width && (dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } } break; case TYPE_U16_STRING: { const uint16_t *arg = a.arg[dp->arg_index].a.a_u16_string; const uint16_t *arg_end; size_t characters; if (has_precision) { /* Use only PRECISION characters, from the left. */ arg_end = arg; characters = 0; for (; precision > 0; precision--) { int count = u16_strmblen (arg_end); if (count == 0) break; if (count < 0) { if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else if (has_width) { /* Use the entire string, and count the number of characters. */ arg_end = arg; characters = 0; for (;;) { int count = u16_strmblen (arg_end); if (count == 0) break; if (count < 0) { if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else { /* Use the entire string. */ arg_end = arg + u16_strlen (arg); /* The number of characters doesn't matter. */ characters = 0; } if (characters < width && !(dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } # if DCHAR_IS_UINT16_T { size_t n = arg_end - arg; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_CPY (result + length, arg, n); length += n; } # else { /* Convert. */ DCHAR_T *converted = result + length; size_t converted_len = allocated - length; # if DCHAR_IS_TCHAR /* Convert from UTF-16 to locale encoding. */ converted = u16_conv_to_encoding (locale_charset (), iconveh_question_mark, arg, arg_end - arg, NULL, converted, &converted_len); # else /* Convert from UTF-16 to UTF-8/UTF-32. */ converted = U16_TO_DCHAR (arg, arg_end - arg, converted, &converted_len); # endif if (converted == NULL) { int saved_errno = errno; if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = saved_errno; return NULL; } if (converted != result + length) { ENSURE_ALLOCATION (xsum (length, converted_len)); DCHAR_CPY (result + length, converted, converted_len); free (converted); } length += converted_len; } # endif if (characters < width && (dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } } break; case TYPE_U32_STRING: { const uint32_t *arg = a.arg[dp->arg_index].a.a_u32_string; const uint32_t *arg_end; size_t characters; if (has_precision) { /* Use only PRECISION characters, from the left. */ arg_end = arg; characters = 0; for (; precision > 0; precision--) { int count = u32_strmblen (arg_end); if (count == 0) break; if (count < 0) { if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else if (has_width) { /* Use the entire string, and count the number of characters. */ arg_end = arg; characters = 0; for (;;) { int count = u32_strmblen (arg_end); if (count == 0) break; if (count < 0) { if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else { /* Use the entire string. */ arg_end = arg + u32_strlen (arg); /* The number of characters doesn't matter. */ characters = 0; } if (characters < width && !(dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } # if DCHAR_IS_UINT32_T { size_t n = arg_end - arg; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_CPY (result + length, arg, n); length += n; } # else { /* Convert. */ DCHAR_T *converted = result + length; size_t converted_len = allocated - length; # if DCHAR_IS_TCHAR /* Convert from UTF-32 to locale encoding. */ converted = u32_conv_to_encoding (locale_charset (), iconveh_question_mark, arg, arg_end - arg, NULL, converted, &converted_len); # else /* Convert from UTF-32 to UTF-8/UTF-16. */ converted = U32_TO_DCHAR (arg, arg_end - arg, converted, &converted_len); # endif if (converted == NULL) { int saved_errno = errno; if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = saved_errno; return NULL; } if (converted != result + length) { ENSURE_ALLOCATION (xsum (length, converted_len)); DCHAR_CPY (result + length, converted, converted_len); free (converted); } length += converted_len; } # endif if (characters < width && (dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } } break; default: abort (); } } #endif #if (!USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || (NEED_PRINTF_DIRECTIVE_LS && !defined IN_LIBINTL)) && HAVE_WCHAR_T else if (dp->conversion == 's' # if WIDE_CHAR_VERSION && a.arg[dp->arg_index].type != TYPE_WIDE_STRING # else && a.arg[dp->arg_index].type == TYPE_WIDE_STRING # endif ) { /* The normal handling of the 's' directive below requires allocating a temporary buffer. The determination of its length (tmp_length), in the case when a precision is specified, below requires a conversion between a char[] string and a wchar_t[] wide string. It could be done, but we have no guarantee that the implementation of sprintf will use the exactly same algorithm. Without this guarantee, it is possible to have buffer overrun bugs. In order to avoid such bugs, we implement the entire processing of the 's' directive ourselves. */ int flags = dp->flags; int has_width; size_t width; int has_precision; size_t precision; has_width = 0; width = 0; if (dp->width_start != dp->width_end) { if (dp->width_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->width_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->width_arg_index].a.a_int; width = arg; if (arg < 0) { /* "A negative field width is taken as a '-' flag followed by a positive field width." */ flags |= FLAG_LEFT; width = -width; } } else { const FCHAR_T *digitp = dp->width_start; do width = xsum (xtimes (width, 10), *digitp++ - '0'); while (digitp != dp->width_end); } has_width = 1; } has_precision = 0; precision = 6; if (dp->precision_start != dp->precision_end) { if (dp->precision_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->precision_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->precision_arg_index].a.a_int; /* "A negative precision is taken as if the precision were omitted." */ if (arg >= 0) { precision = arg; has_precision = 1; } } else { const FCHAR_T *digitp = dp->precision_start + 1; precision = 0; while (digitp != dp->precision_end) precision = xsum (xtimes (precision, 10), *digitp++ - '0'); has_precision = 1; } } # if WIDE_CHAR_VERSION /* %s in vasnwprintf. See the specification of fwprintf. */ { const char *arg = a.arg[dp->arg_index].a.a_string; const char *arg_end; size_t characters; if (has_precision) { /* Use only as many bytes as needed to produce PRECISION wide characters, from the left. */ # if HAVE_MBRTOWC mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif arg_end = arg; characters = 0; for (; precision > 0; precision--) { int count; # if HAVE_MBRTOWC count = mbrlen (arg_end, MB_CUR_MAX, &state); # else count = mblen (arg_end, MB_CUR_MAX); # endif if (count == 0) /* Found the terminating NUL. */ break; if (count < 0) { /* Invalid or incomplete multibyte character. */ if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else if (has_width) { /* Use the entire string, and count the number of wide characters. */ # if HAVE_MBRTOWC mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif arg_end = arg; characters = 0; for (;;) { int count; # if HAVE_MBRTOWC count = mbrlen (arg_end, MB_CUR_MAX, &state); # else count = mblen (arg_end, MB_CUR_MAX); # endif if (count == 0) /* Found the terminating NUL. */ break; if (count < 0) { /* Invalid or incomplete multibyte character. */ if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else { /* Use the entire string. */ arg_end = arg + strlen (arg); /* The number of characters doesn't matter. */ characters = 0; } if (characters < width && !(dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } if (has_precision || has_width) { /* We know the number of wide characters in advance. */ size_t remaining; # if HAVE_MBRTOWC mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif ENSURE_ALLOCATION (xsum (length, characters)); for (remaining = characters; remaining > 0; remaining--) { wchar_t wc; int count; # if HAVE_MBRTOWC count = mbrtowc (&wc, arg, arg_end - arg, &state); # else count = mbtowc (&wc, arg, arg_end - arg); # endif if (count <= 0) /* mbrtowc not consistent with mbrlen, or mbtowc not consistent with mblen. */ abort (); result[length++] = wc; arg += count; } if (!(arg == arg_end)) abort (); } else { # if HAVE_MBRTOWC mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif while (arg < arg_end) { wchar_t wc; int count; # if HAVE_MBRTOWC count = mbrtowc (&wc, arg, arg_end - arg, &state); # else count = mbtowc (&wc, arg, arg_end - arg); # endif if (count <= 0) /* mbrtowc not consistent with mbrlen, or mbtowc not consistent with mblen. */ abort (); ENSURE_ALLOCATION (xsum (length, 1)); result[length++] = wc; arg += count; } } if (characters < width && (dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } } # else /* %ls in vasnprintf. See the specification of fprintf. */ { const wchar_t *arg = a.arg[dp->arg_index].a.a_wide_string; const wchar_t *arg_end; size_t characters; # if !DCHAR_IS_TCHAR /* This code assumes that TCHAR_T is 'char'. */ verify (sizeof (TCHAR_T) == 1); TCHAR_T *tmpsrc; DCHAR_T *tmpdst; size_t tmpdst_len; # endif size_t w; if (has_precision) { /* Use only as many wide characters as needed to produce at most PRECISION bytes, from the left. */ # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif arg_end = arg; characters = 0; while (precision > 0) { char cbuf[64]; /* Assume MB_CUR_MAX <= 64. */ int count; if (*arg_end == 0) /* Found the terminating null wide character. */ break; # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t count = wcrtomb (cbuf, *arg_end, &state); # else count = wctomb (cbuf, *arg_end); # endif if (count < 0) { /* Cannot convert. */ if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } if (precision < count) break; arg_end++; characters += count; precision -= count; } } # if DCHAR_IS_TCHAR else if (has_width) # else else # endif { /* Use the entire string, and count the number of bytes. */ # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif arg_end = arg; characters = 0; for (;;) { char cbuf[64]; /* Assume MB_CUR_MAX <= 64. */ int count; if (*arg_end == 0) /* Found the terminating null wide character. */ break; # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t count = wcrtomb (cbuf, *arg_end, &state); # else count = wctomb (cbuf, *arg_end); # endif if (count < 0) { /* Cannot convert. */ if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end++; characters += count; } } # if DCHAR_IS_TCHAR else { /* Use the entire string. */ arg_end = arg + local_wcslen (arg); /* The number of bytes doesn't matter. */ characters = 0; } # endif # if !DCHAR_IS_TCHAR /* Convert the string into a piece of temporary memory. */ tmpsrc = (TCHAR_T *) malloc (characters * sizeof (TCHAR_T)); if (tmpsrc == NULL) goto out_of_memory; { TCHAR_T *tmpptr = tmpsrc; size_t remaining; # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif for (remaining = characters; remaining > 0; ) { char cbuf[64]; /* Assume MB_CUR_MAX <= 64. */ int count; if (*arg == 0) abort (); # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t count = wcrtomb (cbuf, *arg, &state); # else count = wctomb (cbuf, *arg); # endif if (count <= 0) /* Inconsistency. */ abort (); memcpy (tmpptr, cbuf, count); tmpptr += count; arg++; remaining -= count; } if (!(arg == arg_end)) abort (); } /* Convert from TCHAR_T[] to DCHAR_T[]. */ tmpdst = DCHAR_CONV_FROM_ENCODING (locale_charset (), iconveh_question_mark, tmpsrc, characters, NULL, NULL, &tmpdst_len); if (tmpdst == NULL) { int saved_errno = errno; free (tmpsrc); if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = saved_errno; return NULL; } free (tmpsrc); # endif if (has_width) { # if ENABLE_UNISTDIO /* Outside POSIX, it's preferable to compare the width against the number of _characters_ of the converted value. */ w = DCHAR_MBSNLEN (result + length, characters); # else /* The width is compared against the number of _bytes_ of the converted value, says POSIX. */ w = characters; # endif } else /* w doesn't matter. */ w = 0; if (w < width && !(dp->flags & FLAG_LEFT)) { size_t n = width - w; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } # if DCHAR_IS_TCHAR if (has_precision || has_width) { /* We know the number of bytes in advance. */ size_t remaining; # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif ENSURE_ALLOCATION (xsum (length, characters)); for (remaining = characters; remaining > 0; ) { char cbuf[64]; /* Assume MB_CUR_MAX <= 64. */ int count; if (*arg == 0) abort (); # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t count = wcrtomb (cbuf, *arg, &state); # else count = wctomb (cbuf, *arg); # endif if (count <= 0) /* Inconsistency. */ abort (); memcpy (result + length, cbuf, count); length += count; arg++; remaining -= count; } if (!(arg == arg_end)) abort (); } else { # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif while (arg < arg_end) { char cbuf[64]; /* Assume MB_CUR_MAX <= 64. */ int count; if (*arg == 0) abort (); # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t count = wcrtomb (cbuf, *arg, &state); # else count = wctomb (cbuf, *arg); # endif if (count <= 0) { /* Cannot convert. */ if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } ENSURE_ALLOCATION (xsum (length, count)); memcpy (result + length, cbuf, count); length += count; arg++; } } # else ENSURE_ALLOCATION (xsum (length, tmpdst_len)); DCHAR_CPY (result + length, tmpdst, tmpdst_len); free (tmpdst); length += tmpdst_len; # endif if (w < width && (dp->flags & FLAG_LEFT)) { size_t n = width - w; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } } # endif } #endif #if (NEED_PRINTF_DIRECTIVE_A || NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_DOUBLE) && !defined IN_LIBINTL else if ((dp->conversion == 'a' || dp->conversion == 'A') # if !(NEED_PRINTF_DIRECTIVE_A || (NEED_PRINTF_LONG_DOUBLE && NEED_PRINTF_DOUBLE)) && (0 # if NEED_PRINTF_DOUBLE || a.arg[dp->arg_index].type == TYPE_DOUBLE # endif # if NEED_PRINTF_LONG_DOUBLE || a.arg[dp->arg_index].type == TYPE_LONGDOUBLE # endif ) # endif ) { arg_type type = a.arg[dp->arg_index].type; int flags = dp->flags; size_t width; int has_precision; size_t precision; size_t tmp_length; size_t count; DCHAR_T tmpbuf[700]; DCHAR_T *tmp; DCHAR_T *pad_ptr; DCHAR_T *p; width = 0; if (dp->width_start != dp->width_end) { if (dp->width_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->width_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->width_arg_index].a.a_int; width = arg; if (arg < 0) { /* "A negative field width is taken as a '-' flag followed by a positive field width." */ flags |= FLAG_LEFT; width = -width; } } else { const FCHAR_T *digitp = dp->width_start; do width = xsum (xtimes (width, 10), *digitp++ - '0'); while (digitp != dp->width_end); } } has_precision = 0; precision = 0; if (dp->precision_start != dp->precision_end) { if (dp->precision_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->precision_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->precision_arg_index].a.a_int; /* "A negative precision is taken as if the precision were omitted." */ if (arg >= 0) { precision = arg; has_precision = 1; } } else { const FCHAR_T *digitp = dp->precision_start + 1; precision = 0; while (digitp != dp->precision_end) precision = xsum (xtimes (precision, 10), *digitp++ - '0'); has_precision = 1; } } /* Allocate a temporary buffer of sufficient size. */ if (type == TYPE_LONGDOUBLE) tmp_length = (unsigned int) ((LDBL_DIG + 1) * 0.831 /* decimal -> hexadecimal */ ) + 1; /* turn floor into ceil */ else tmp_length = (unsigned int) ((DBL_DIG + 1) * 0.831 /* decimal -> hexadecimal */ ) + 1; /* turn floor into ceil */ if (tmp_length < precision) tmp_length = precision; /* Account for sign, decimal point etc. */ tmp_length = xsum (tmp_length, 12); if (tmp_length < width) tmp_length = width; tmp_length = xsum (tmp_length, 1); /* account for trailing NUL */ if (tmp_length <= sizeof (tmpbuf) / sizeof (DCHAR_T)) tmp = tmpbuf; else { size_t tmp_memsize = xtimes (tmp_length, sizeof (DCHAR_T)); if (size_overflow_p (tmp_memsize)) /* Overflow, would lead to out of memory. */ goto out_of_memory; tmp = (DCHAR_T *) malloc (tmp_memsize); if (tmp == NULL) /* Out of memory. */ goto out_of_memory; } pad_ptr = NULL; p = tmp; if (type == TYPE_LONGDOUBLE) { # if NEED_PRINTF_DIRECTIVE_A || NEED_PRINTF_LONG_DOUBLE long double arg = a.arg[dp->arg_index].a.a_longdouble; if (isnanl (arg)) { if (dp->conversion == 'A') { *p++ = 'N'; *p++ = 'A'; *p++ = 'N'; } else { *p++ = 'n'; *p++ = 'a'; *p++ = 'n'; } } else { int sign = 0; DECL_LONG_DOUBLE_ROUNDING BEGIN_LONG_DOUBLE_ROUNDING (); if (signbit (arg)) /* arg < 0.0L or negative zero */ { sign = -1; arg = -arg; } if (sign < 0) *p++ = '-'; else if (flags & FLAG_SHOWSIGN) *p++ = '+'; else if (flags & FLAG_SPACE) *p++ = ' '; if (arg > 0.0L && arg + arg == arg) { if (dp->conversion == 'A') { *p++ = 'I'; *p++ = 'N'; *p++ = 'F'; } else { *p++ = 'i'; *p++ = 'n'; *p++ = 'f'; } } else { int exponent; long double mantissa; if (arg > 0.0L) mantissa = printf_frexpl (arg, &exponent); else { exponent = 0; mantissa = 0.0L; } if (has_precision && precision < (unsigned int) ((LDBL_DIG + 1) * 0.831) + 1) { /* Round the mantissa. */ long double tail = mantissa; size_t q; for (q = precision; ; q--) { int digit = (int) tail; tail -= digit; if (q == 0) { if (digit & 1 ? tail >= 0.5L : tail > 0.5L) tail = 1 - tail; else tail = - tail; break; } tail *= 16.0L; } if (tail != 0.0L) for (q = precision; q > 0; q--) tail *= 0.0625L; mantissa += tail; } *p++ = '0'; *p++ = dp->conversion - 'A' + 'X'; pad_ptr = p; { int digit; digit = (int) mantissa; mantissa -= digit; *p++ = '0' + digit; if ((flags & FLAG_ALT) || mantissa > 0.0L || precision > 0) { *p++ = decimal_point_char (); /* This loop terminates because we assume that FLT_RADIX is a power of 2. */ while (mantissa > 0.0L) { mantissa *= 16.0L; digit = (int) mantissa; mantissa -= digit; *p++ = digit + (digit < 10 ? '0' : dp->conversion - 10); if (precision > 0) precision--; } while (precision > 0) { *p++ = '0'; precision--; } } } *p++ = dp->conversion - 'A' + 'P'; # if WIDE_CHAR_VERSION { static const wchar_t decimal_format[] = { '%', '+', 'd', '\0' }; SNPRINTF (p, 6 + 1, decimal_format, exponent); } while (*p != '\0') p++; # else if (sizeof (DCHAR_T) == 1) { sprintf ((char *) p, "%+d", exponent); while (*p != '\0') p++; } else { char expbuf[6 + 1]; const char *ep; sprintf (expbuf, "%+d", exponent); for (ep = expbuf; (*p = *ep) != '\0'; ep++) p++; } # endif } END_LONG_DOUBLE_ROUNDING (); } # else abort (); # endif } else { # if NEED_PRINTF_DIRECTIVE_A || NEED_PRINTF_DOUBLE double arg = a.arg[dp->arg_index].a.a_double; if (isnand (arg)) { if (dp->conversion == 'A') { *p++ = 'N'; *p++ = 'A'; *p++ = 'N'; } else { *p++ = 'n'; *p++ = 'a'; *p++ = 'n'; } } else { int sign = 0; if (signbit (arg)) /* arg < 0.0 or negative zero */ { sign = -1; arg = -arg; } if (sign < 0) *p++ = '-'; else if (flags & FLAG_SHOWSIGN) *p++ = '+'; else if (flags & FLAG_SPACE) *p++ = ' '; if (arg > 0.0 && arg + arg == arg) { if (dp->conversion == 'A') { *p++ = 'I'; *p++ = 'N'; *p++ = 'F'; } else { *p++ = 'i'; *p++ = 'n'; *p++ = 'f'; } } else { int exponent; double mantissa; if (arg > 0.0) mantissa = printf_frexp (arg, &exponent); else { exponent = 0; mantissa = 0.0; } if (has_precision && precision < (unsigned int) ((DBL_DIG + 1) * 0.831) + 1) { /* Round the mantissa. */ double tail = mantissa; size_t q; for (q = precision; ; q--) { int digit = (int) tail; tail -= digit; if (q == 0) { if (digit & 1 ? tail >= 0.5 : tail > 0.5) tail = 1 - tail; else tail = - tail; break; } tail *= 16.0; } if (tail != 0.0) for (q = precision; q > 0; q--) tail *= 0.0625; mantissa += tail; } *p++ = '0'; *p++ = dp->conversion - 'A' + 'X'; pad_ptr = p; { int digit; digit = (int) mantissa; mantissa -= digit; *p++ = '0' + digit; if ((flags & FLAG_ALT) || mantissa > 0.0 || precision > 0) { *p++ = decimal_point_char (); /* This loop terminates because we assume that FLT_RADIX is a power of 2. */ while (mantissa > 0.0) { mantissa *= 16.0; digit = (int) mantissa; mantissa -= digit; *p++ = digit + (digit < 10 ? '0' : dp->conversion - 10); if (precision > 0) precision--; } while (precision > 0) { *p++ = '0'; precision--; } } } *p++ = dp->conversion - 'A' + 'P'; # if WIDE_CHAR_VERSION { static const wchar_t decimal_format[] = { '%', '+', 'd', '\0' }; SNPRINTF (p, 6 + 1, decimal_format, exponent); } while (*p != '\0') p++; # else if (sizeof (DCHAR_T) == 1) { sprintf ((char *) p, "%+d", exponent); while (*p != '\0') p++; } else { char expbuf[6 + 1]; const char *ep; sprintf (expbuf, "%+d", exponent); for (ep = expbuf; (*p = *ep) != '\0'; ep++) p++; } # endif } } # else abort (); # endif } /* The generated string now extends from tmp to p, with the zero padding insertion point being at pad_ptr. */ count = p - tmp; if (count < width) { size_t pad = width - count; DCHAR_T *end = p + pad; if (flags & FLAG_LEFT) { /* Pad with spaces on the right. */ for (; pad > 0; pad--) *p++ = ' '; } else if ((flags & FLAG_ZERO) && pad_ptr != NULL) { /* Pad with zeroes. */ DCHAR_T *q = end; while (p > pad_ptr) *--q = *--p; for (; pad > 0; pad--) *p++ = '0'; } else { /* Pad with spaces on the left. */ DCHAR_T *q = end; while (p > tmp) *--q = *--p; for (; pad > 0; pad--) *p++ = ' '; } p = end; } count = p - tmp; if (count >= tmp_length) /* tmp_length was incorrectly calculated - fix the code above! */ abort (); /* Make room for the result. */ if (count >= allocated - length) { size_t n = xsum (length, count); ENSURE_ALLOCATION (n); } /* Append the result. */ memcpy (result + length, tmp, count * sizeof (DCHAR_T)); if (tmp != tmpbuf) free (tmp); length += count; } #endif #if (NEED_PRINTF_INFINITE_DOUBLE || NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_LONG_DOUBLE || NEED_PRINTF_LONG_DOUBLE) && !defined IN_LIBINTL else if ((dp->conversion == 'f' || dp->conversion == 'F' || dp->conversion == 'e' || dp->conversion == 'E' || dp->conversion == 'g' || dp->conversion == 'G' || dp->conversion == 'a' || dp->conversion == 'A') && (0 # if NEED_PRINTF_DOUBLE || a.arg[dp->arg_index].type == TYPE_DOUBLE # elif NEED_PRINTF_INFINITE_DOUBLE || (a.arg[dp->arg_index].type == TYPE_DOUBLE /* The systems (mingw) which produce wrong output for Inf, -Inf, and NaN also do so for -0.0. Therefore we treat this case here as well. */ && is_infinite_or_zero (a.arg[dp->arg_index].a.a_double)) # endif # if NEED_PRINTF_LONG_DOUBLE || a.arg[dp->arg_index].type == TYPE_LONGDOUBLE # elif NEED_PRINTF_INFINITE_LONG_DOUBLE || (a.arg[dp->arg_index].type == TYPE_LONGDOUBLE /* Some systems produce wrong output for Inf, -Inf, and NaN. Some systems in this category (IRIX 5.3) also do so for -0.0. Therefore we treat this case here as well. */ && is_infinite_or_zerol (a.arg[dp->arg_index].a.a_longdouble)) # endif )) { # if (NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_DOUBLE) && (NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_INFINITE_LONG_DOUBLE) arg_type type = a.arg[dp->arg_index].type; # endif int flags = dp->flags; size_t width; size_t count; int has_precision; size_t precision; size_t tmp_length; DCHAR_T tmpbuf[700]; DCHAR_T *tmp; DCHAR_T *pad_ptr; DCHAR_T *p; width = 0; if (dp->width_start != dp->width_end) { if (dp->width_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->width_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->width_arg_index].a.a_int; width = arg; if (arg < 0) { /* "A negative field width is taken as a '-' flag followed by a positive field width." */ flags |= FLAG_LEFT; width = -width; } } else { const FCHAR_T *digitp = dp->width_start; do width = xsum (xtimes (width, 10), *digitp++ - '0'); while (digitp != dp->width_end); } } has_precision = 0; precision = 0; if (dp->precision_start != dp->precision_end) { if (dp->precision_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->precision_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->precision_arg_index].a.a_int; /* "A negative precision is taken as if the precision were omitted." */ if (arg >= 0) { precision = arg; has_precision = 1; } } else { const FCHAR_T *digitp = dp->precision_start + 1; precision = 0; while (digitp != dp->precision_end) precision = xsum (xtimes (precision, 10), *digitp++ - '0'); has_precision = 1; } } /* POSIX specifies the default precision to be 6 for %f, %F, %e, %E, but not for %g, %G. Implementations appear to use the same default precision also for %g, %G. But for %a, %A, the default precision is 0. */ if (!has_precision) if (!(dp->conversion == 'a' || dp->conversion == 'A')) precision = 6; /* Allocate a temporary buffer of sufficient size. */ # if NEED_PRINTF_DOUBLE && NEED_PRINTF_LONG_DOUBLE tmp_length = (type == TYPE_LONGDOUBLE ? LDBL_DIG + 1 : DBL_DIG + 1); # elif NEED_PRINTF_INFINITE_DOUBLE && NEED_PRINTF_LONG_DOUBLE tmp_length = (type == TYPE_LONGDOUBLE ? LDBL_DIG + 1 : 0); # elif NEED_PRINTF_LONG_DOUBLE tmp_length = LDBL_DIG + 1; # elif NEED_PRINTF_DOUBLE tmp_length = DBL_DIG + 1; # else tmp_length = 0; # endif if (tmp_length < precision) tmp_length = precision; # if NEED_PRINTF_LONG_DOUBLE # if NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_DOUBLE if (type == TYPE_LONGDOUBLE) # endif if (dp->conversion == 'f' || dp->conversion == 'F') { long double arg = a.arg[dp->arg_index].a.a_longdouble; if (!(isnanl (arg) || arg + arg == arg)) { /* arg is finite and nonzero. */ int exponent = floorlog10l (arg < 0 ? -arg : arg); if (exponent >= 0 && tmp_length < exponent + precision) tmp_length = exponent + precision; } } # endif # if NEED_PRINTF_DOUBLE # if NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_INFINITE_LONG_DOUBLE if (type == TYPE_DOUBLE) # endif if (dp->conversion == 'f' || dp->conversion == 'F') { double arg = a.arg[dp->arg_index].a.a_double; if (!(isnand (arg) || arg + arg == arg)) { /* arg is finite and nonzero. */ int exponent = floorlog10 (arg < 0 ? -arg : arg); if (exponent >= 0 && tmp_length < exponent + precision) tmp_length = exponent + precision; } } # endif /* Account for sign, decimal point etc. */ tmp_length = xsum (tmp_length, 12); if (tmp_length < width) tmp_length = width; tmp_length = xsum (tmp_length, 1); /* account for trailing NUL */ if (tmp_length <= sizeof (tmpbuf) / sizeof (DCHAR_T)) tmp = tmpbuf; else { size_t tmp_memsize = xtimes (tmp_length, sizeof (DCHAR_T)); if (size_overflow_p (tmp_memsize)) /* Overflow, would lead to out of memory. */ goto out_of_memory; tmp = (DCHAR_T *) malloc (tmp_memsize); if (tmp == NULL) /* Out of memory. */ goto out_of_memory; } pad_ptr = NULL; p = tmp; # if NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_INFINITE_LONG_DOUBLE # if NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_DOUBLE if (type == TYPE_LONGDOUBLE) # endif { long double arg = a.arg[dp->arg_index].a.a_longdouble; if (isnanl (arg)) { if (dp->conversion >= 'A' && dp->conversion <= 'Z') { *p++ = 'N'; *p++ = 'A'; *p++ = 'N'; } else { *p++ = 'n'; *p++ = 'a'; *p++ = 'n'; } } else { int sign = 0; DECL_LONG_DOUBLE_ROUNDING BEGIN_LONG_DOUBLE_ROUNDING (); if (signbit (arg)) /* arg < 0.0L or negative zero */ { sign = -1; arg = -arg; } if (sign < 0) *p++ = '-'; else if (flags & FLAG_SHOWSIGN) *p++ = '+'; else if (flags & FLAG_SPACE) *p++ = ' '; if (arg > 0.0L && arg + arg == arg) { if (dp->conversion >= 'A' && dp->conversion <= 'Z') { *p++ = 'I'; *p++ = 'N'; *p++ = 'F'; } else { *p++ = 'i'; *p++ = 'n'; *p++ = 'f'; } } else { # if NEED_PRINTF_LONG_DOUBLE pad_ptr = p; if (dp->conversion == 'f' || dp->conversion == 'F') { char *digits; size_t ndigits; digits = scale10_round_decimal_long_double (arg, precision); if (digits == NULL) { END_LONG_DOUBLE_ROUNDING (); goto out_of_memory; } ndigits = strlen (digits); if (ndigits > precision) do { --ndigits; *p++ = digits[ndigits]; } while (ndigits > precision); else *p++ = '0'; /* Here ndigits <= precision. */ if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > ndigits; precision--) *p++ = '0'; while (ndigits > 0) { --ndigits; *p++ = digits[ndigits]; } } free (digits); } else if (dp->conversion == 'e' || dp->conversion == 'E') { int exponent; if (arg == 0.0L) { exponent = 0; *p++ = '0'; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > 0; precision--) *p++ = '0'; } } else { /* arg > 0.0L. */ int adjusted; char *digits; size_t ndigits; exponent = floorlog10l (arg); adjusted = 0; for (;;) { digits = scale10_round_decimal_long_double (arg, (int)precision - exponent); if (digits == NULL) { END_LONG_DOUBLE_ROUNDING (); goto out_of_memory; } ndigits = strlen (digits); if (ndigits == precision + 1) break; if (ndigits < precision || ndigits > precision + 2) /* The exponent was not guessed precisely enough. */ abort (); if (adjusted) /* None of two values of exponent is the right one. Prevent an endless loop. */ abort (); free (digits); if (ndigits == precision) exponent -= 1; else exponent += 1; adjusted = 1; } /* Here ndigits = precision+1. */ if (is_borderline (digits, precision)) { /* Maybe the exponent guess was too high and a smaller exponent can be reached by turning a 10...0 into 9...9x. */ char *digits2 = scale10_round_decimal_long_double (arg, (int)precision - exponent + 1); if (digits2 == NULL) { free (digits); END_LONG_DOUBLE_ROUNDING (); goto out_of_memory; } if (strlen (digits2) == precision + 1) { free (digits); digits = digits2; exponent -= 1; } else free (digits2); } /* Here ndigits = precision+1. */ *p++ = digits[--ndigits]; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); while (ndigits > 0) { --ndigits; *p++ = digits[ndigits]; } } free (digits); } *p++ = dp->conversion; /* 'e' or 'E' */ # if WIDE_CHAR_VERSION { static const wchar_t decimal_format[] = { '%', '+', '.', '2', 'd', '\0' }; SNPRINTF (p, 6 + 1, decimal_format, exponent); } while (*p != '\0') p++; # else if (sizeof (DCHAR_T) == 1) { sprintf ((char *) p, "%+.2d", exponent); while (*p != '\0') p++; } else { char expbuf[6 + 1]; const char *ep; sprintf (expbuf, "%+.2d", exponent); for (ep = expbuf; (*p = *ep) != '\0'; ep++) p++; } # endif } else if (dp->conversion == 'g' || dp->conversion == 'G') { if (precision == 0) precision = 1; /* precision >= 1. */ if (arg == 0.0L) /* The exponent is 0, >= -4, < precision. Use fixed-point notation. */ { size_t ndigits = precision; /* Number of trailing zeroes that have to be dropped. */ size_t nzeroes = (flags & FLAG_ALT ? 0 : precision - 1); --ndigits; *p++ = '0'; if ((flags & FLAG_ALT) || ndigits > nzeroes) { *p++ = decimal_point_char (); while (ndigits > nzeroes) { --ndigits; *p++ = '0'; } } } else { /* arg > 0.0L. */ int exponent; int adjusted; char *digits; size_t ndigits; size_t nzeroes; exponent = floorlog10l (arg); adjusted = 0; for (;;) { digits = scale10_round_decimal_long_double (arg, (int)(precision - 1) - exponent); if (digits == NULL) { END_LONG_DOUBLE_ROUNDING (); goto out_of_memory; } ndigits = strlen (digits); if (ndigits == precision) break; if (ndigits < precision - 1 || ndigits > precision + 1) /* The exponent was not guessed precisely enough. */ abort (); if (adjusted) /* None of two values of exponent is the right one. Prevent an endless loop. */ abort (); free (digits); if (ndigits < precision) exponent -= 1; else exponent += 1; adjusted = 1; } /* Here ndigits = precision. */ if (is_borderline (digits, precision - 1)) { /* Maybe the exponent guess was too high and a smaller exponent can be reached by turning a 10...0 into 9...9x. */ char *digits2 = scale10_round_decimal_long_double (arg, (int)(precision - 1) - exponent + 1); if (digits2 == NULL) { free (digits); END_LONG_DOUBLE_ROUNDING (); goto out_of_memory; } if (strlen (digits2) == precision) { free (digits); digits = digits2; exponent -= 1; } else free (digits2); } /* Here ndigits = precision. */ /* Determine the number of trailing zeroes that have to be dropped. */ nzeroes = 0; if ((flags & FLAG_ALT) == 0) while (nzeroes < ndigits && digits[nzeroes] == '0') nzeroes++; /* The exponent is now determined. */ if (exponent >= -4 && exponent < (long)precision) { /* Fixed-point notation: max(exponent,0)+1 digits, then the decimal point, then the remaining digits without trailing zeroes. */ if (exponent >= 0) { size_t ecount = exponent + 1; /* Note: count <= precision = ndigits. */ for (; ecount > 0; ecount--) *p++ = digits[--ndigits]; if ((flags & FLAG_ALT) || ndigits > nzeroes) { *p++ = decimal_point_char (); while (ndigits > nzeroes) { --ndigits; *p++ = digits[ndigits]; } } } else { size_t ecount = -exponent - 1; *p++ = '0'; *p++ = decimal_point_char (); for (; ecount > 0; ecount--) *p++ = '0'; while (ndigits > nzeroes) { --ndigits; *p++ = digits[ndigits]; } } } else { /* Exponential notation. */ *p++ = digits[--ndigits]; if ((flags & FLAG_ALT) || ndigits > nzeroes) { *p++ = decimal_point_char (); while (ndigits > nzeroes) { --ndigits; *p++ = digits[ndigits]; } } *p++ = dp->conversion - 'G' + 'E'; /* 'e' or 'E' */ # if WIDE_CHAR_VERSION { static const wchar_t decimal_format[] = { '%', '+', '.', '2', 'd', '\0' }; SNPRINTF (p, 6 + 1, decimal_format, exponent); } while (*p != '\0') p++; # else if (sizeof (DCHAR_T) == 1) { sprintf ((char *) p, "%+.2d", exponent); while (*p != '\0') p++; } else { char expbuf[6 + 1]; const char *ep; sprintf (expbuf, "%+.2d", exponent); for (ep = expbuf; (*p = *ep) != '\0'; ep++) p++; } # endif } free (digits); } } else abort (); # else /* arg is finite. */ if (!(arg == 0.0L)) abort (); pad_ptr = p; if (dp->conversion == 'f' || dp->conversion == 'F') { *p++ = '0'; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > 0; precision--) *p++ = '0'; } } else if (dp->conversion == 'e' || dp->conversion == 'E') { *p++ = '0'; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > 0; precision--) *p++ = '0'; } *p++ = dp->conversion; /* 'e' or 'E' */ *p++ = '+'; *p++ = '0'; *p++ = '0'; } else if (dp->conversion == 'g' || dp->conversion == 'G') { *p++ = '0'; if (flags & FLAG_ALT) { size_t ndigits = (precision > 0 ? precision - 1 : 0); *p++ = decimal_point_char (); for (; ndigits > 0; --ndigits) *p++ = '0'; } } else if (dp->conversion == 'a' || dp->conversion == 'A') { *p++ = '0'; *p++ = dp->conversion - 'A' + 'X'; pad_ptr = p; *p++ = '0'; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > 0; precision--) *p++ = '0'; } *p++ = dp->conversion - 'A' + 'P'; *p++ = '+'; *p++ = '0'; } else abort (); # endif } END_LONG_DOUBLE_ROUNDING (); } } # if NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_DOUBLE else # endif # endif # if NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_DOUBLE { double arg = a.arg[dp->arg_index].a.a_double; if (isnand (arg)) { if (dp->conversion >= 'A' && dp->conversion <= 'Z') { *p++ = 'N'; *p++ = 'A'; *p++ = 'N'; } else { *p++ = 'n'; *p++ = 'a'; *p++ = 'n'; } } else { int sign = 0; if (signbit (arg)) /* arg < 0.0 or negative zero */ { sign = -1; arg = -arg; } if (sign < 0) *p++ = '-'; else if (flags & FLAG_SHOWSIGN) *p++ = '+'; else if (flags & FLAG_SPACE) *p++ = ' '; if (arg > 0.0 && arg + arg == arg) { if (dp->conversion >= 'A' && dp->conversion <= 'Z') { *p++ = 'I'; *p++ = 'N'; *p++ = 'F'; } else { *p++ = 'i'; *p++ = 'n'; *p++ = 'f'; } } else { # if NEED_PRINTF_DOUBLE pad_ptr = p; if (dp->conversion == 'f' || dp->conversion == 'F') { char *digits; size_t ndigits; digits = scale10_round_decimal_double (arg, precision); if (digits == NULL) goto out_of_memory; ndigits = strlen (digits); if (ndigits > precision) do { --ndigits; *p++ = digits[ndigits]; } while (ndigits > precision); else *p++ = '0'; /* Here ndigits <= precision. */ if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > ndigits; precision--) *p++ = '0'; while (ndigits > 0) { --ndigits; *p++ = digits[ndigits]; } } free (digits); } else if (dp->conversion == 'e' || dp->conversion == 'E') { int exponent; if (arg == 0.0) { exponent = 0; *p++ = '0'; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > 0; precision--) *p++ = '0'; } } else { /* arg > 0.0. */ int adjusted; char *digits; size_t ndigits; exponent = floorlog10 (arg); adjusted = 0; for (;;) { digits = scale10_round_decimal_double (arg, (int)precision - exponent); if (digits == NULL) goto out_of_memory; ndigits = strlen (digits); if (ndigits == precision + 1) break; if (ndigits < precision || ndigits > precision + 2) /* The exponent was not guessed precisely enough. */ abort (); if (adjusted) /* None of two values of exponent is the right one. Prevent an endless loop. */ abort (); free (digits); if (ndigits == precision) exponent -= 1; else exponent += 1; adjusted = 1; } /* Here ndigits = precision+1. */ if (is_borderline (digits, precision)) { /* Maybe the exponent guess was too high and a smaller exponent can be reached by turning a 10...0 into 9...9x. */ char *digits2 = scale10_round_decimal_double (arg, (int)precision - exponent + 1); if (digits2 == NULL) { free (digits); goto out_of_memory; } if (strlen (digits2) == precision + 1) { free (digits); digits = digits2; exponent -= 1; } else free (digits2); } /* Here ndigits = precision+1. */ *p++ = digits[--ndigits]; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); while (ndigits > 0) { --ndigits; *p++ = digits[ndigits]; } } free (digits); } *p++ = dp->conversion; /* 'e' or 'E' */ # if WIDE_CHAR_VERSION { static const wchar_t decimal_format[] = /* Produce the same number of exponent digits as the native printf implementation. */ # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ { '%', '+', '.', '3', 'd', '\0' }; # else { '%', '+', '.', '2', 'd', '\0' }; # endif SNPRINTF (p, 6 + 1, decimal_format, exponent); } while (*p != '\0') p++; # else { static const char decimal_format[] = /* Produce the same number of exponent digits as the native printf implementation. */ # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ "%+.3d"; # else "%+.2d"; # endif if (sizeof (DCHAR_T) == 1) { sprintf ((char *) p, decimal_format, exponent); while (*p != '\0') p++; } else { char expbuf[6 + 1]; const char *ep; sprintf (expbuf, decimal_format, exponent); for (ep = expbuf; (*p = *ep) != '\0'; ep++) p++; } } # endif } else if (dp->conversion == 'g' || dp->conversion == 'G') { if (precision == 0) precision = 1; /* precision >= 1. */ if (arg == 0.0) /* The exponent is 0, >= -4, < precision. Use fixed-point notation. */ { size_t ndigits = precision; /* Number of trailing zeroes that have to be dropped. */ size_t nzeroes = (flags & FLAG_ALT ? 0 : precision - 1); --ndigits; *p++ = '0'; if ((flags & FLAG_ALT) || ndigits > nzeroes) { *p++ = decimal_point_char (); while (ndigits > nzeroes) { --ndigits; *p++ = '0'; } } } else { /* arg > 0.0. */ int exponent; int adjusted; char *digits; size_t ndigits; size_t nzeroes; exponent = floorlog10 (arg); adjusted = 0; for (;;) { digits = scale10_round_decimal_double (arg, (int)(precision - 1) - exponent); if (digits == NULL) goto out_of_memory; ndigits = strlen (digits); if (ndigits == precision) break; if (ndigits < precision - 1 || ndigits > precision + 1) /* The exponent was not guessed precisely enough. */ abort (); if (adjusted) /* None of two values of exponent is the right one. Prevent an endless loop. */ abort (); free (digits); if (ndigits < precision) exponent -= 1; else exponent += 1; adjusted = 1; } /* Here ndigits = precision. */ if (is_borderline (digits, precision - 1)) { /* Maybe the exponent guess was too high and a smaller exponent can be reached by turning a 10...0 into 9...9x. */ char *digits2 = scale10_round_decimal_double (arg, (int)(precision - 1) - exponent + 1); if (digits2 == NULL) { free (digits); goto out_of_memory; } if (strlen (digits2) == precision) { free (digits); digits = digits2; exponent -= 1; } else free (digits2); } /* Here ndigits = precision. */ /* Determine the number of trailing zeroes that have to be dropped. */ nzeroes = 0; if ((flags & FLAG_ALT) == 0) while (nzeroes < ndigits && digits[nzeroes] == '0') nzeroes++; /* The exponent is now determined. */ if (exponent >= -4 && exponent < (long)precision) { /* Fixed-point notation: max(exponent,0)+1 digits, then the decimal point, then the remaining digits without trailing zeroes. */ if (exponent >= 0) { size_t ecount = exponent + 1; /* Note: ecount <= precision = ndigits. */ for (; ecount > 0; ecount--) *p++ = digits[--ndigits]; if ((flags & FLAG_ALT) || ndigits > nzeroes) { *p++ = decimal_point_char (); while (ndigits > nzeroes) { --ndigits; *p++ = digits[ndigits]; } } } else { size_t ecount = -exponent - 1; *p++ = '0'; *p++ = decimal_point_char (); for (; ecount > 0; ecount--) *p++ = '0'; while (ndigits > nzeroes) { --ndigits; *p++ = digits[ndigits]; } } } else { /* Exponential notation. */ *p++ = digits[--ndigits]; if ((flags & FLAG_ALT) || ndigits > nzeroes) { *p++ = decimal_point_char (); while (ndigits > nzeroes) { --ndigits; *p++ = digits[ndigits]; } } *p++ = dp->conversion - 'G' + 'E'; /* 'e' or 'E' */ # if WIDE_CHAR_VERSION { static const wchar_t decimal_format[] = /* Produce the same number of exponent digits as the native printf implementation. */ # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ { '%', '+', '.', '3', 'd', '\0' }; # else { '%', '+', '.', '2', 'd', '\0' }; # endif SNPRINTF (p, 6 + 1, decimal_format, exponent); } while (*p != '\0') p++; # else { static const char decimal_format[] = /* Produce the same number of exponent digits as the native printf implementation. */ # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ "%+.3d"; # else "%+.2d"; # endif if (sizeof (DCHAR_T) == 1) { sprintf ((char *) p, decimal_format, exponent); while (*p != '\0') p++; } else { char expbuf[6 + 1]; const char *ep; sprintf (expbuf, decimal_format, exponent); for (ep = expbuf; (*p = *ep) != '\0'; ep++) p++; } } # endif } free (digits); } } else abort (); # else /* arg is finite. */ if (!(arg == 0.0)) abort (); pad_ptr = p; if (dp->conversion == 'f' || dp->conversion == 'F') { *p++ = '0'; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > 0; precision--) *p++ = '0'; } } else if (dp->conversion == 'e' || dp->conversion == 'E') { *p++ = '0'; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > 0; precision--) *p++ = '0'; } *p++ = dp->conversion; /* 'e' or 'E' */ *p++ = '+'; /* Produce the same number of exponent digits as the native printf implementation. */ # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ *p++ = '0'; # endif *p++ = '0'; *p++ = '0'; } else if (dp->conversion == 'g' || dp->conversion == 'G') { *p++ = '0'; if (flags & FLAG_ALT) { size_t ndigits = (precision > 0 ? precision - 1 : 0); *p++ = decimal_point_char (); for (; ndigits > 0; --ndigits) *p++ = '0'; } } else abort (); # endif } } } # endif /* The generated string now extends from tmp to p, with the zero padding insertion point being at pad_ptr. */ count = p - tmp; if (count < width) { size_t pad = width - count; DCHAR_T *end = p + pad; if (flags & FLAG_LEFT) { /* Pad with spaces on the right. */ for (; pad > 0; pad--) *p++ = ' '; } else if ((flags & FLAG_ZERO) && pad_ptr != NULL) { /* Pad with zeroes. */ DCHAR_T *q = end; while (p > pad_ptr) *--q = *--p; for (; pad > 0; pad--) *p++ = '0'; } else { /* Pad with spaces on the left. */ DCHAR_T *q = end; while (p > tmp) *--q = *--p; for (; pad > 0; pad--) *p++ = ' '; } p = end; } count = p - tmp; if (count >= tmp_length) /* tmp_length was incorrectly calculated - fix the code above! */ abort (); /* Make room for the result. */ if (count >= allocated - length) { size_t n = xsum (length, count); ENSURE_ALLOCATION (n); } /* Append the result. */ memcpy (result + length, tmp, count * sizeof (DCHAR_T)); if (tmp != tmpbuf) free (tmp); length += count; } #endif else { arg_type type = a.arg[dp->arg_index].type; int flags = dp->flags; #if !DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_LEFTADJUST || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION int has_width; #endif #if !USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || !DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_LEFTADJUST || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION size_t width; #endif #if !USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || NEED_PRINTF_UNBOUNDED_PRECISION int has_precision; size_t precision; #endif #if NEED_PRINTF_UNBOUNDED_PRECISION int prec_ourselves; #else # define prec_ourselves 0 #endif #if NEED_PRINTF_FLAG_LEFTADJUST # define pad_ourselves 1 #elif !DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION int pad_ourselves; #else # define pad_ourselves 0 #endif TCHAR_T *fbp; unsigned int prefix_count; int prefixes[2] IF_LINT (= { 0 }); int orig_errno; #if !USE_SNPRINTF size_t tmp_length; TCHAR_T tmpbuf[700]; TCHAR_T *tmp; #endif #if !DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_LEFTADJUST || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION has_width = 0; #endif #if !USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || !DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_LEFTADJUST || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION width = 0; if (dp->width_start != dp->width_end) { if (dp->width_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->width_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->width_arg_index].a.a_int; width = arg; if (arg < 0) { /* "A negative field width is taken as a '-' flag followed by a positive field width." */ flags |= FLAG_LEFT; width = -width; } } else { const FCHAR_T *digitp = dp->width_start; do width = xsum (xtimes (width, 10), *digitp++ - '0'); while (digitp != dp->width_end); } #if !DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_LEFTADJUST || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION has_width = 1; #endif } #endif #if !USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || NEED_PRINTF_UNBOUNDED_PRECISION has_precision = 0; precision = 6; if (dp->precision_start != dp->precision_end) { if (dp->precision_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->precision_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->precision_arg_index].a.a_int; /* "A negative precision is taken as if the precision were omitted." */ if (arg >= 0) { precision = arg; has_precision = 1; } } else { const FCHAR_T *digitp = dp->precision_start + 1; precision = 0; while (digitp != dp->precision_end) precision = xsum (xtimes (precision, 10), *digitp++ - '0'); has_precision = 1; } } #endif /* Decide whether to handle the precision ourselves. */ #if NEED_PRINTF_UNBOUNDED_PRECISION switch (dp->conversion) { case 'd': case 'i': case 'u': case 'o': case 'x': case 'X': case 'p': prec_ourselves = has_precision && (precision > 0); break; default: prec_ourselves = 0; break; } #endif /* Decide whether to perform the padding ourselves. */ #if !NEED_PRINTF_FLAG_LEFTADJUST && (!DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION) switch (dp->conversion) { # if !DCHAR_IS_TCHAR || ENABLE_UNISTDIO /* If we need conversion from TCHAR_T[] to DCHAR_T[], we need to perform the padding after this conversion. Functions with unistdio extensions perform the padding based on character count rather than element count. */ case 'c': case 's': # endif # if NEED_PRINTF_FLAG_ZERO case 'f': case 'F': case 'e': case 'E': case 'g': case 'G': case 'a': case 'A': # endif pad_ourselves = 1; break; default: pad_ourselves = prec_ourselves; break; } #endif #if !USE_SNPRINTF /* Allocate a temporary buffer of sufficient size for calling sprintf. */ tmp_length = MAX_ROOM_NEEDED (&a, dp->arg_index, dp->conversion, type, flags, width, has_precision, precision, pad_ourselves); if (tmp_length <= sizeof (tmpbuf) / sizeof (TCHAR_T)) tmp = tmpbuf; else { size_t tmp_memsize = xtimes (tmp_length, sizeof (TCHAR_T)); if (size_overflow_p (tmp_memsize)) /* Overflow, would lead to out of memory. */ goto out_of_memory; tmp = (TCHAR_T *) malloc (tmp_memsize); if (tmp == NULL) /* Out of memory. */ goto out_of_memory; } #endif /* Construct the format string for calling snprintf or sprintf. */ fbp = buf; *fbp++ = '%'; #if NEED_PRINTF_FLAG_GROUPING /* The underlying implementation doesn't support the ' flag. Produce no grouping characters in this case; this is acceptable because the grouping is locale dependent. */ #else if (flags & FLAG_GROUP) *fbp++ = '\''; #endif if (flags & FLAG_LEFT) *fbp++ = '-'; if (flags & FLAG_SHOWSIGN) *fbp++ = '+'; if (flags & FLAG_SPACE) *fbp++ = ' '; if (flags & FLAG_ALT) *fbp++ = '#'; #if __GLIBC__ >= 2 && !defined __UCLIBC__ if (flags & FLAG_LOCALIZED) *fbp++ = 'I'; #endif if (!pad_ourselves) { if (flags & FLAG_ZERO) *fbp++ = '0'; if (dp->width_start != dp->width_end) { size_t n = dp->width_end - dp->width_start; /* The width specification is known to consist only of standard ASCII characters. */ if (sizeof (FCHAR_T) == sizeof (TCHAR_T)) { memcpy (fbp, dp->width_start, n * sizeof (TCHAR_T)); fbp += n; } else { const FCHAR_T *mp = dp->width_start; do *fbp++ = *mp++; while (--n > 0); } } } if (!prec_ourselves) { if (dp->precision_start != dp->precision_end) { size_t n = dp->precision_end - dp->precision_start; /* The precision specification is known to consist only of standard ASCII characters. */ if (sizeof (FCHAR_T) == sizeof (TCHAR_T)) { memcpy (fbp, dp->precision_start, n * sizeof (TCHAR_T)); fbp += n; } else { const FCHAR_T *mp = dp->precision_start; do *fbp++ = *mp++; while (--n > 0); } } } switch (type) { #if HAVE_LONG_LONG_INT case TYPE_LONGLONGINT: case TYPE_ULONGLONGINT: # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ *fbp++ = 'I'; *fbp++ = '6'; *fbp++ = '4'; break; # else *fbp++ = 'l'; # endif #endif /*FALLTHROUGH*/ case TYPE_LONGINT: case TYPE_ULONGINT: #if HAVE_WINT_T case TYPE_WIDE_CHAR: #endif #if HAVE_WCHAR_T case TYPE_WIDE_STRING: #endif *fbp++ = 'l'; break; case TYPE_LONGDOUBLE: *fbp++ = 'L'; break; default: break; } #if NEED_PRINTF_DIRECTIVE_F if (dp->conversion == 'F') *fbp = 'f'; else #endif *fbp = dp->conversion; #if USE_SNPRINTF # if !(((__GLIBC__ > 2 || (__GLIBC__ == 2 && __GLIBC_MINOR__ >= 3)) && !defined __UCLIBC__) || ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__)) fbp[1] = '%'; fbp[2] = 'n'; fbp[3] = '\0'; # else /* On glibc2 systems from glibc >= 2.3 - probably also older ones - we know that snprintf's return value conforms to ISO C 99: the tests gl_SNPRINTF_RETVAL_C99 and gl_SNPRINTF_TRUNCATION_C99 pass. Therefore we can avoid using %n in this situation. On glibc2 systems from 2004-10-18 or newer, the use of %n in format strings in writable memory may crash the program (if compiled with _FORTIFY_SOURCE=2), so we should avoid it in this situation. */ /* On native Windows systems (such as mingw), we can avoid using %n because: - Although the gl_SNPRINTF_TRUNCATION_C99 test fails, snprintf does not write more than the specified number of bytes. (snprintf (buf, 3, "%d %d", 4567, 89) writes '4', '5', '6' into buf, not '4', '5', '\0'.) - Although the gl_SNPRINTF_RETVAL_C99 test fails, snprintf allows us to recognize the case of an insufficient buffer size: it returns -1 in this case. On native Windows systems (such as mingw) where the OS is Windows Vista, the use of %n in format strings by default crashes the program. See and So we should avoid %n in this situation. */ fbp[1] = '\0'; # endif #else fbp[1] = '\0'; #endif /* Construct the arguments for calling snprintf or sprintf. */ prefix_count = 0; if (!pad_ourselves && dp->width_arg_index != ARG_NONE) { if (!(a.arg[dp->width_arg_index].type == TYPE_INT)) abort (); prefixes[prefix_count++] = a.arg[dp->width_arg_index].a.a_int; } if (!prec_ourselves && dp->precision_arg_index != ARG_NONE) { if (!(a.arg[dp->precision_arg_index].type == TYPE_INT)) abort (); prefixes[prefix_count++] = a.arg[dp->precision_arg_index].a.a_int; } #if USE_SNPRINTF /* The SNPRINTF result is appended after result[0..length]. The latter is an array of DCHAR_T; SNPRINTF appends an array of TCHAR_T to it. This is possible because sizeof (TCHAR_T) divides sizeof (DCHAR_T) and alignof (TCHAR_T) <= alignof (DCHAR_T). */ # define TCHARS_PER_DCHAR (sizeof (DCHAR_T) / sizeof (TCHAR_T)) /* Ensure that maxlen below will be >= 2. Needed on BeOS, where an snprintf() with maxlen==1 acts like sprintf(). */ ENSURE_ALLOCATION (xsum (length, (2 + TCHARS_PER_DCHAR - 1) / TCHARS_PER_DCHAR)); /* Prepare checking whether snprintf returns the count via %n. */ *(TCHAR_T *) (result + length) = '\0'; #endif orig_errno = errno; for (;;) { int count = -1; #if USE_SNPRINTF int retcount = 0; size_t maxlen = allocated - length; /* SNPRINTF can fail if its second argument is > INT_MAX. */ if (maxlen > INT_MAX / TCHARS_PER_DCHAR) maxlen = INT_MAX / TCHARS_PER_DCHAR; maxlen = maxlen * TCHARS_PER_DCHAR; # define SNPRINTF_BUF(arg) \ switch (prefix_count) \ { \ case 0: \ retcount = SNPRINTF ((TCHAR_T *) (result + length), \ maxlen, buf, \ arg, &count); \ break; \ case 1: \ retcount = SNPRINTF ((TCHAR_T *) (result + length), \ maxlen, buf, \ prefixes[0], arg, &count); \ break; \ case 2: \ retcount = SNPRINTF ((TCHAR_T *) (result + length), \ maxlen, buf, \ prefixes[0], prefixes[1], arg, \ &count); \ break; \ default: \ abort (); \ } #else # define SNPRINTF_BUF(arg) \ switch (prefix_count) \ { \ case 0: \ count = sprintf (tmp, buf, arg); \ break; \ case 1: \ count = sprintf (tmp, buf, prefixes[0], arg); \ break; \ case 2: \ count = sprintf (tmp, buf, prefixes[0], prefixes[1],\ arg); \ break; \ default: \ abort (); \ } #endif errno = 0; switch (type) { case TYPE_SCHAR: { int arg = a.arg[dp->arg_index].a.a_schar; SNPRINTF_BUF (arg); } break; case TYPE_UCHAR: { unsigned int arg = a.arg[dp->arg_index].a.a_uchar; SNPRINTF_BUF (arg); } break; case TYPE_SHORT: { int arg = a.arg[dp->arg_index].a.a_short; SNPRINTF_BUF (arg); } break; case TYPE_USHORT: { unsigned int arg = a.arg[dp->arg_index].a.a_ushort; SNPRINTF_BUF (arg); } break; case TYPE_INT: { int arg = a.arg[dp->arg_index].a.a_int; SNPRINTF_BUF (arg); } break; case TYPE_UINT: { unsigned int arg = a.arg[dp->arg_index].a.a_uint; SNPRINTF_BUF (arg); } break; case TYPE_LONGINT: { long int arg = a.arg[dp->arg_index].a.a_longint; SNPRINTF_BUF (arg); } break; case TYPE_ULONGINT: { unsigned long int arg = a.arg[dp->arg_index].a.a_ulongint; SNPRINTF_BUF (arg); } break; #if HAVE_LONG_LONG_INT case TYPE_LONGLONGINT: { long long int arg = a.arg[dp->arg_index].a.a_longlongint; SNPRINTF_BUF (arg); } break; case TYPE_ULONGLONGINT: { unsigned long long int arg = a.arg[dp->arg_index].a.a_ulonglongint; SNPRINTF_BUF (arg); } break; #endif case TYPE_DOUBLE: { double arg = a.arg[dp->arg_index].a.a_double; SNPRINTF_BUF (arg); } break; case TYPE_LONGDOUBLE: { long double arg = a.arg[dp->arg_index].a.a_longdouble; SNPRINTF_BUF (arg); } break; case TYPE_CHAR: { int arg = a.arg[dp->arg_index].a.a_char; SNPRINTF_BUF (arg); } break; #if HAVE_WINT_T case TYPE_WIDE_CHAR: { wint_t arg = a.arg[dp->arg_index].a.a_wide_char; SNPRINTF_BUF (arg); } break; #endif case TYPE_STRING: { const char *arg = a.arg[dp->arg_index].a.a_string; SNPRINTF_BUF (arg); } break; #if HAVE_WCHAR_T case TYPE_WIDE_STRING: { const wchar_t *arg = a.arg[dp->arg_index].a.a_wide_string; SNPRINTF_BUF (arg); } break; #endif case TYPE_POINTER: { void *arg = a.arg[dp->arg_index].a.a_pointer; SNPRINTF_BUF (arg); } break; default: abort (); } #if USE_SNPRINTF /* Portability: Not all implementations of snprintf() are ISO C 99 compliant. Determine the number of bytes that snprintf() has produced or would have produced. */ if (count >= 0) { /* Verify that snprintf() has NUL-terminated its result. */ if (count < maxlen && ((TCHAR_T *) (result + length)) [count] != '\0') abort (); /* Portability hack. */ if (retcount > count) count = retcount; } else { /* snprintf() doesn't understand the '%n' directive. */ if (fbp[1] != '\0') { /* Don't use the '%n' directive; instead, look at the snprintf() return value. */ fbp[1] = '\0'; continue; } else { /* Look at the snprintf() return value. */ if (retcount < 0) { # if !HAVE_SNPRINTF_RETVAL_C99 /* HP-UX 10.20 snprintf() is doubly deficient: It doesn't understand the '%n' directive, *and* it returns -1 (rather than the length that would have been required) when the buffer is too small. But a failure at this point can also come from other reasons than a too small buffer, such as an invalid wide string argument to the %ls directive, or possibly an invalid floating-point argument. */ size_t tmp_length = MAX_ROOM_NEEDED (&a, dp->arg_index, dp->conversion, type, flags, width, has_precision, precision, pad_ourselves); if (maxlen < tmp_length) { /* Make more room. But try to do through this reallocation only once. */ size_t bigger_need = xsum (length, xsum (tmp_length, TCHARS_PER_DCHAR - 1) / TCHARS_PER_DCHAR); /* And always grow proportionally. (There may be several arguments, each needing a little more room than the previous one.) */ size_t bigger_need2 = xsum (xtimes (allocated, 2), 12); if (bigger_need < bigger_need2) bigger_need = bigger_need2; ENSURE_ALLOCATION (bigger_need); continue; } # endif } else count = retcount; } } #endif /* Attempt to handle failure. */ if (count < 0) { /* SNPRINTF or sprintf failed. Save and use the errno that it has set, if any. */ int saved_errno = errno; if (saved_errno == 0) { if (dp->conversion == 'c' || dp->conversion == 's') saved_errno = EILSEQ; else saved_errno = EINVAL; } if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = saved_errno; return NULL; } #if USE_SNPRINTF /* Handle overflow of the allocated buffer. If such an overflow occurs, a C99 compliant snprintf() returns a count >= maxlen. However, a non-compliant snprintf() function returns only count = maxlen - 1. To cover both cases, test whether count >= maxlen - 1. */ if ((unsigned int) count + 1 >= maxlen) { /* If maxlen already has attained its allowed maximum, allocating more memory will not increase maxlen. Instead of looping, bail out. */ if (maxlen == INT_MAX / TCHARS_PER_DCHAR) goto overflow; else { /* Need at least (count + 1) * sizeof (TCHAR_T) bytes. (The +1 is for the trailing NUL.) But ask for (count + 2) * sizeof (TCHAR_T) bytes, so that in the next round, we likely get maxlen > (unsigned int) count + 1 and so we don't get here again. And allocate proportionally, to avoid looping eternally if snprintf() reports a too small count. */ size_t n = xmax (xsum (length, ((unsigned int) count + 2 + TCHARS_PER_DCHAR - 1) / TCHARS_PER_DCHAR), xtimes (allocated, 2)); ENSURE_ALLOCATION (n); continue; } } #endif #if NEED_PRINTF_UNBOUNDED_PRECISION if (prec_ourselves) { /* Handle the precision. */ TCHAR_T *prec_ptr = # if USE_SNPRINTF (TCHAR_T *) (result + length); # else tmp; # endif size_t prefix_count; size_t move; prefix_count = 0; /* Put the additional zeroes after the sign. */ if (count >= 1 && (*prec_ptr == '-' || *prec_ptr == '+' || *prec_ptr == ' ')) prefix_count = 1; /* Put the additional zeroes after the 0x prefix if (flags & FLAG_ALT) || (dp->conversion == 'p'). */ else if (count >= 2 && prec_ptr[0] == '0' && (prec_ptr[1] == 'x' || prec_ptr[1] == 'X')) prefix_count = 2; move = count - prefix_count; if (precision > move) { /* Insert zeroes. */ size_t insert = precision - move; TCHAR_T *prec_end; # if USE_SNPRINTF size_t n = xsum (length, (count + insert + TCHARS_PER_DCHAR - 1) / TCHARS_PER_DCHAR); length += (count + TCHARS_PER_DCHAR - 1) / TCHARS_PER_DCHAR; ENSURE_ALLOCATION (n); length -= (count + TCHARS_PER_DCHAR - 1) / TCHARS_PER_DCHAR; prec_ptr = (TCHAR_T *) (result + length); # endif prec_end = prec_ptr + count; prec_ptr += prefix_count; while (prec_end > prec_ptr) { prec_end--; prec_end[insert] = prec_end[0]; } prec_end += insert; do *--prec_end = '0'; while (prec_end > prec_ptr); count += insert; } } #endif #if !USE_SNPRINTF if (count >= tmp_length) /* tmp_length was incorrectly calculated - fix the code above! */ abort (); #endif #if !DCHAR_IS_TCHAR /* Convert from TCHAR_T[] to DCHAR_T[]. */ if (dp->conversion == 'c' || dp->conversion == 's') { /* type = TYPE_CHAR or TYPE_WIDE_CHAR or TYPE_STRING TYPE_WIDE_STRING. The result string is not certainly ASCII. */ const TCHAR_T *tmpsrc; DCHAR_T *tmpdst; size_t tmpdst_len; /* This code assumes that TCHAR_T is 'char'. */ verify (sizeof (TCHAR_T) == 1); # if USE_SNPRINTF tmpsrc = (TCHAR_T *) (result + length); # else tmpsrc = tmp; # endif tmpdst = DCHAR_CONV_FROM_ENCODING (locale_charset (), iconveh_question_mark, tmpsrc, count, NULL, NULL, &tmpdst_len); if (tmpdst == NULL) { int saved_errno = errno; if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = saved_errno; return NULL; } ENSURE_ALLOCATION (xsum (length, tmpdst_len)); DCHAR_CPY (result + length, tmpdst, tmpdst_len); free (tmpdst); count = tmpdst_len; } else { /* The result string is ASCII. Simple 1:1 conversion. */ # if USE_SNPRINTF /* If sizeof (DCHAR_T) == sizeof (TCHAR_T), it's a no-op conversion, in-place on the array starting at (result + length). */ if (sizeof (DCHAR_T) != sizeof (TCHAR_T)) # endif { const TCHAR_T *tmpsrc; DCHAR_T *tmpdst; size_t n; # if USE_SNPRINTF if (result == resultbuf) { tmpsrc = (TCHAR_T *) (result + length); /* ENSURE_ALLOCATION will not move tmpsrc (because it's part of resultbuf). */ ENSURE_ALLOCATION (xsum (length, count)); } else { /* ENSURE_ALLOCATION will move the array (because it uses realloc(). */ ENSURE_ALLOCATION (xsum (length, count)); tmpsrc = (TCHAR_T *) (result + length); } # else tmpsrc = tmp; ENSURE_ALLOCATION (xsum (length, count)); # endif tmpdst = result + length; /* Copy backwards, because of overlapping. */ tmpsrc += count; tmpdst += count; for (n = count; n > 0; n--) *--tmpdst = *--tmpsrc; } } #endif #if DCHAR_IS_TCHAR && !USE_SNPRINTF /* Make room for the result. */ if (count > allocated - length) { /* Need at least count elements. But allocate proportionally. */ size_t n = xmax (xsum (length, count), xtimes (allocated, 2)); ENSURE_ALLOCATION (n); } #endif /* Here count <= allocated - length. */ /* Perform padding. */ #if !DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_LEFTADJUST || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION if (pad_ourselves && has_width) { size_t w; # if ENABLE_UNISTDIO /* Outside POSIX, it's preferable to compare the width against the number of _characters_ of the converted value. */ w = DCHAR_MBSNLEN (result + length, count); # else /* The width is compared against the number of _bytes_ of the converted value, says POSIX. */ w = count; # endif if (w < width) { size_t pad = width - w; /* Make room for the result. */ if (xsum (count, pad) > allocated - length) { /* Need at least count + pad elements. But allocate proportionally. */ size_t n = xmax (xsum3 (length, count, pad), xtimes (allocated, 2)); # if USE_SNPRINTF length += count; ENSURE_ALLOCATION (n); length -= count; # else ENSURE_ALLOCATION (n); # endif } /* Here count + pad <= allocated - length. */ { # if !DCHAR_IS_TCHAR || USE_SNPRINTF DCHAR_T * const rp = result + length; # else DCHAR_T * const rp = tmp; # endif DCHAR_T *p = rp + count; DCHAR_T *end = p + pad; DCHAR_T *pad_ptr; # if !DCHAR_IS_TCHAR || ENABLE_UNISTDIO if (dp->conversion == 'c' || dp->conversion == 's') /* No zero-padding for string directives. */ pad_ptr = NULL; else # endif { pad_ptr = (*rp == '-' ? rp + 1 : rp); /* No zero-padding of "inf" and "nan". */ if ((*pad_ptr >= 'A' && *pad_ptr <= 'Z') || (*pad_ptr >= 'a' && *pad_ptr <= 'z')) pad_ptr = NULL; } /* The generated string now extends from rp to p, with the zero padding insertion point being at pad_ptr. */ count = count + pad; /* = end - rp */ if (flags & FLAG_LEFT) { /* Pad with spaces on the right. */ for (; pad > 0; pad--) *p++ = ' '; } else if ((flags & FLAG_ZERO) && pad_ptr != NULL) { /* Pad with zeroes. */ DCHAR_T *q = end; while (p > pad_ptr) *--q = *--p; for (; pad > 0; pad--) *p++ = '0'; } else { /* Pad with spaces on the left. */ DCHAR_T *q = end; while (p > rp) *--q = *--p; for (; pad > 0; pad--) *p++ = ' '; } } } } #endif /* Here still count <= allocated - length. */ #if !DCHAR_IS_TCHAR || USE_SNPRINTF /* The snprintf() result did fit. */ #else /* Append the sprintf() result. */ memcpy (result + length, tmp, count * sizeof (DCHAR_T)); #endif #if !USE_SNPRINTF if (tmp != tmpbuf) free (tmp); #endif #if NEED_PRINTF_DIRECTIVE_F if (dp->conversion == 'F') { /* Convert the %f result to upper case for %F. */ DCHAR_T *rp = result + length; size_t rc; for (rc = count; rc > 0; rc--, rp++) if (*rp >= 'a' && *rp <= 'z') *rp = *rp - 'a' + 'A'; } #endif length += count; break; } errno = orig_errno; #undef pad_ourselves #undef prec_ourselves } } } /* Add the final NUL. */ ENSURE_ALLOCATION (xsum (length, 1)); result[length] = '\0'; if (result != resultbuf && length + 1 < allocated) { /* Shrink the allocated memory if possible. */ DCHAR_T *memory; memory = (DCHAR_T *) realloc (result, (length + 1) * sizeof (DCHAR_T)); if (memory != NULL) result = memory; } if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); *lengthp = length; /* Note that we can produce a big string of a length > INT_MAX. POSIX says that snprintf() fails with errno = EOVERFLOW in this case, but that's only because snprintf() returns an 'int'. This function does not have this limitation. */ return result; #if USE_SNPRINTF overflow: if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EOVERFLOW; return NULL; #endif out_of_memory: if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); out_of_memory_1: CLEANUP (); errno = ENOMEM; return NULL; } } #undef MAX_ROOM_NEEDED #undef TCHARS_PER_DCHAR #undef SNPRINTF #undef USE_SNPRINTF #undef DCHAR_SET #undef DCHAR_CPY #undef PRINTF_PARSE #undef DIRECTIVES #undef DIRECTIVE #undef DCHAR_IS_TCHAR #undef TCHAR_T #undef DCHAR_T #undef FCHAR_T #undef VASNPRINTF gnuastro-0.2.33-8a3b/bootstrapped/lib/printf-parse.c0000644000175000017500000005317113004436754017164 00000000000000/* Formatted output to strings. Copyright (C) 1999-2000, 2002-2003, 2006-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* This file can be parametrized with the following macros: CHAR_T The element type of the format string. CHAR_T_ONLY_ASCII Set to 1 to enable verification that all characters in the format string are ASCII. DIRECTIVE Structure denoting a format directive. Depends on CHAR_T. DIRECTIVES Structure denoting the set of format directives of a format string. Depends on CHAR_T. PRINTF_PARSE Function that parses a format string. Depends on CHAR_T. STATIC Set to 'static' to declare the function static. ENABLE_UNISTDIO Set to 1 to enable the unistdio extensions. */ #ifndef PRINTF_PARSE # include #endif /* Specification. */ #ifndef PRINTF_PARSE # include "printf-parse.h" #endif /* Default parameters. */ #ifndef PRINTF_PARSE # define PRINTF_PARSE printf_parse # define CHAR_T char # define DIRECTIVE char_directive # define DIRECTIVES char_directives #endif /* Get size_t, NULL. */ #include /* Get intmax_t. */ #if defined IN_LIBINTL || defined IN_LIBASPRINTF # if HAVE_STDINT_H_WITH_UINTMAX # include # endif # if HAVE_INTTYPES_H_WITH_UINTMAX # include # endif #else # include #endif /* malloc(), realloc(), free(). */ #include /* memcpy(). */ #include /* errno. */ #include /* Checked size_t computations. */ #include "xsize.h" #if CHAR_T_ONLY_ASCII /* c_isascii(). */ # include "c-ctype.h" #endif #ifdef STATIC STATIC #endif int PRINTF_PARSE (const CHAR_T *format, DIRECTIVES *d, arguments *a) { const CHAR_T *cp = format; /* pointer into format */ size_t arg_posn = 0; /* number of regular arguments consumed */ size_t d_allocated; /* allocated elements of d->dir */ size_t a_allocated; /* allocated elements of a->arg */ size_t max_width_length = 0; size_t max_precision_length = 0; d->count = 0; d_allocated = N_DIRECT_ALLOC_DIRECTIVES; d->dir = d->direct_alloc_dir; a->count = 0; a_allocated = N_DIRECT_ALLOC_ARGUMENTS; a->arg = a->direct_alloc_arg; #define REGISTER_ARG(_index_,_type_) \ { \ size_t n = (_index_); \ if (n >= a_allocated) \ { \ size_t memory_size; \ argument *memory; \ \ a_allocated = xtimes (a_allocated, 2); \ if (a_allocated <= n) \ a_allocated = xsum (n, 1); \ memory_size = xtimes (a_allocated, sizeof (argument)); \ if (size_overflow_p (memory_size)) \ /* Overflow, would lead to out of memory. */ \ goto out_of_memory; \ memory = (argument *) (a->arg != a->direct_alloc_arg \ ? realloc (a->arg, memory_size) \ : malloc (memory_size)); \ if (memory == NULL) \ /* Out of memory. */ \ goto out_of_memory; \ if (a->arg == a->direct_alloc_arg) \ memcpy (memory, a->arg, a->count * sizeof (argument)); \ a->arg = memory; \ } \ while (a->count <= n) \ a->arg[a->count++].type = TYPE_NONE; \ if (a->arg[n].type == TYPE_NONE) \ a->arg[n].type = (_type_); \ else if (a->arg[n].type != (_type_)) \ /* Ambiguous type for positional argument. */ \ goto error; \ } while (*cp != '\0') { CHAR_T c = *cp++; if (c == '%') { size_t arg_index = ARG_NONE; DIRECTIVE *dp = &d->dir[d->count]; /* pointer to next directive */ /* Initialize the next directive. */ dp->dir_start = cp - 1; dp->flags = 0; dp->width_start = NULL; dp->width_end = NULL; dp->width_arg_index = ARG_NONE; dp->precision_start = NULL; dp->precision_end = NULL; dp->precision_arg_index = ARG_NONE; dp->arg_index = ARG_NONE; /* Test for positional argument. */ if (*cp >= '0' && *cp <= '9') { const CHAR_T *np; for (np = cp; *np >= '0' && *np <= '9'; np++) ; if (*np == '$') { size_t n = 0; for (np = cp; *np >= '0' && *np <= '9'; np++) n = xsum (xtimes (n, 10), *np - '0'); if (n == 0) /* Positional argument 0. */ goto error; if (size_overflow_p (n)) /* n too large, would lead to out of memory later. */ goto error; arg_index = n - 1; cp = np + 1; } } /* Read the flags. */ for (;;) { if (*cp == '\'') { dp->flags |= FLAG_GROUP; cp++; } else if (*cp == '-') { dp->flags |= FLAG_LEFT; cp++; } else if (*cp == '+') { dp->flags |= FLAG_SHOWSIGN; cp++; } else if (*cp == ' ') { dp->flags |= FLAG_SPACE; cp++; } else if (*cp == '#') { dp->flags |= FLAG_ALT; cp++; } else if (*cp == '0') { dp->flags |= FLAG_ZERO; cp++; } #if __GLIBC__ >= 2 && !defined __UCLIBC__ else if (*cp == 'I') { dp->flags |= FLAG_LOCALIZED; cp++; } #endif else break; } /* Parse the field width. */ if (*cp == '*') { dp->width_start = cp; cp++; dp->width_end = cp; if (max_width_length < 1) max_width_length = 1; /* Test for positional argument. */ if (*cp >= '0' && *cp <= '9') { const CHAR_T *np; for (np = cp; *np >= '0' && *np <= '9'; np++) ; if (*np == '$') { size_t n = 0; for (np = cp; *np >= '0' && *np <= '9'; np++) n = xsum (xtimes (n, 10), *np - '0'); if (n == 0) /* Positional argument 0. */ goto error; if (size_overflow_p (n)) /* n too large, would lead to out of memory later. */ goto error; dp->width_arg_index = n - 1; cp = np + 1; } } if (dp->width_arg_index == ARG_NONE) { dp->width_arg_index = arg_posn++; if (dp->width_arg_index == ARG_NONE) /* arg_posn wrapped around. */ goto error; } REGISTER_ARG (dp->width_arg_index, TYPE_INT); } else if (*cp >= '0' && *cp <= '9') { size_t width_length; dp->width_start = cp; for (; *cp >= '0' && *cp <= '9'; cp++) ; dp->width_end = cp; width_length = dp->width_end - dp->width_start; if (max_width_length < width_length) max_width_length = width_length; } /* Parse the precision. */ if (*cp == '.') { cp++; if (*cp == '*') { dp->precision_start = cp - 1; cp++; dp->precision_end = cp; if (max_precision_length < 2) max_precision_length = 2; /* Test for positional argument. */ if (*cp >= '0' && *cp <= '9') { const CHAR_T *np; for (np = cp; *np >= '0' && *np <= '9'; np++) ; if (*np == '$') { size_t n = 0; for (np = cp; *np >= '0' && *np <= '9'; np++) n = xsum (xtimes (n, 10), *np - '0'); if (n == 0) /* Positional argument 0. */ goto error; if (size_overflow_p (n)) /* n too large, would lead to out of memory later. */ goto error; dp->precision_arg_index = n - 1; cp = np + 1; } } if (dp->precision_arg_index == ARG_NONE) { dp->precision_arg_index = arg_posn++; if (dp->precision_arg_index == ARG_NONE) /* arg_posn wrapped around. */ goto error; } REGISTER_ARG (dp->precision_arg_index, TYPE_INT); } else { size_t precision_length; dp->precision_start = cp - 1; for (; *cp >= '0' && *cp <= '9'; cp++) ; dp->precision_end = cp; precision_length = dp->precision_end - dp->precision_start; if (max_precision_length < precision_length) max_precision_length = precision_length; } } { arg_type type; /* Parse argument type/size specifiers. */ { int flags = 0; for (;;) { if (*cp == 'h') { flags |= (1 << (flags & 1)); cp++; } else if (*cp == 'L') { flags |= 4; cp++; } else if (*cp == 'l') { flags += 8; cp++; } else if (*cp == 'j') { if (sizeof (intmax_t) > sizeof (long)) { /* intmax_t = long long */ flags += 16; } else if (sizeof (intmax_t) > sizeof (int)) { /* intmax_t = long */ flags += 8; } cp++; } else if (*cp == 'z' || *cp == 'Z') { /* 'z' is standardized in ISO C 99, but glibc uses 'Z' because the warning facility in gcc-2.95.2 understands only 'Z' (see gcc-2.95.2/gcc/c-common.c:1784). */ if (sizeof (size_t) > sizeof (long)) { /* size_t = long long */ flags += 16; } else if (sizeof (size_t) > sizeof (int)) { /* size_t = long */ flags += 8; } cp++; } else if (*cp == 't') { if (sizeof (ptrdiff_t) > sizeof (long)) { /* ptrdiff_t = long long */ flags += 16; } else if (sizeof (ptrdiff_t) > sizeof (int)) { /* ptrdiff_t = long */ flags += 8; } cp++; } #if defined __APPLE__ && defined __MACH__ /* On Mac OS X 10.3, PRIdMAX is defined as "qd". We cannot change it to "lld" because PRIdMAX must also be understood by the system's printf routines. */ else if (*cp == 'q') { if (64 / 8 > sizeof (long)) { /* int64_t = long long */ flags += 16; } else { /* int64_t = long */ flags += 8; } cp++; } #endif #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* On native Windows, PRIdMAX is defined as "I64d". We cannot change it to "lld" because PRIdMAX must also be understood by the system's printf routines. */ else if (*cp == 'I' && cp[1] == '6' && cp[2] == '4') { if (64 / 8 > sizeof (long)) { /* __int64 = long long */ flags += 16; } else { /* __int64 = long */ flags += 8; } cp += 3; } #endif else break; } /* Read the conversion character. */ c = *cp++; switch (c) { case 'd': case 'i': #if HAVE_LONG_LONG_INT /* If 'long long' exists and is larger than 'long': */ if (flags >= 16 || (flags & 4)) type = TYPE_LONGLONGINT; else #endif /* If 'long long' exists and is the same as 'long', we parse "lld" into TYPE_LONGINT. */ if (flags >= 8) type = TYPE_LONGINT; else if (flags & 2) type = TYPE_SCHAR; else if (flags & 1) type = TYPE_SHORT; else type = TYPE_INT; break; case 'o': case 'u': case 'x': case 'X': #if HAVE_LONG_LONG_INT /* If 'long long' exists and is larger than 'long': */ if (flags >= 16 || (flags & 4)) type = TYPE_ULONGLONGINT; else #endif /* If 'unsigned long long' exists and is the same as 'unsigned long', we parse "llu" into TYPE_ULONGINT. */ if (flags >= 8) type = TYPE_ULONGINT; else if (flags & 2) type = TYPE_UCHAR; else if (flags & 1) type = TYPE_USHORT; else type = TYPE_UINT; break; case 'f': case 'F': case 'e': case 'E': case 'g': case 'G': case 'a': case 'A': if (flags >= 16 || (flags & 4)) type = TYPE_LONGDOUBLE; else type = TYPE_DOUBLE; break; case 'c': if (flags >= 8) #if HAVE_WINT_T type = TYPE_WIDE_CHAR; #else goto error; #endif else type = TYPE_CHAR; break; #if HAVE_WINT_T case 'C': type = TYPE_WIDE_CHAR; c = 'c'; break; #endif case 's': if (flags >= 8) #if HAVE_WCHAR_T type = TYPE_WIDE_STRING; #else goto error; #endif else type = TYPE_STRING; break; #if HAVE_WCHAR_T case 'S': type = TYPE_WIDE_STRING; c = 's'; break; #endif case 'p': type = TYPE_POINTER; break; case 'n': #if HAVE_LONG_LONG_INT /* If 'long long' exists and is larger than 'long': */ if (flags >= 16 || (flags & 4)) type = TYPE_COUNT_LONGLONGINT_POINTER; else #endif /* If 'long long' exists and is the same as 'long', we parse "lln" into TYPE_COUNT_LONGINT_POINTER. */ if (flags >= 8) type = TYPE_COUNT_LONGINT_POINTER; else if (flags & 2) type = TYPE_COUNT_SCHAR_POINTER; else if (flags & 1) type = TYPE_COUNT_SHORT_POINTER; else type = TYPE_COUNT_INT_POINTER; break; #if ENABLE_UNISTDIO /* The unistdio extensions. */ case 'U': if (flags >= 16) type = TYPE_U32_STRING; else if (flags >= 8) type = TYPE_U16_STRING; else type = TYPE_U8_STRING; break; #endif case '%': type = TYPE_NONE; break; default: /* Unknown conversion character. */ goto error; } } if (type != TYPE_NONE) { dp->arg_index = arg_index; if (dp->arg_index == ARG_NONE) { dp->arg_index = arg_posn++; if (dp->arg_index == ARG_NONE) /* arg_posn wrapped around. */ goto error; } REGISTER_ARG (dp->arg_index, type); } dp->conversion = c; dp->dir_end = cp; } d->count++; if (d->count >= d_allocated) { size_t memory_size; DIRECTIVE *memory; d_allocated = xtimes (d_allocated, 2); memory_size = xtimes (d_allocated, sizeof (DIRECTIVE)); if (size_overflow_p (memory_size)) /* Overflow, would lead to out of memory. */ goto out_of_memory; memory = (DIRECTIVE *) (d->dir != d->direct_alloc_dir ? realloc (d->dir, memory_size) : malloc (memory_size)); if (memory == NULL) /* Out of memory. */ goto out_of_memory; if (d->dir == d->direct_alloc_dir) memcpy (memory, d->dir, d->count * sizeof (DIRECTIVE)); d->dir = memory; } } #if CHAR_T_ONLY_ASCII else if (!c_isascii (c)) { /* Non-ASCII character. Not supported. */ goto error; } #endif } d->dir[d->count].dir_start = cp; d->max_width_length = max_width_length; d->max_precision_length = max_precision_length; return 0; error: if (a->arg != a->direct_alloc_arg) free (a->arg); if (d->dir != d->direct_alloc_dir) free (d->dir); errno = EINVAL; return -1; out_of_memory: if (a->arg != a->direct_alloc_arg) free (a->arg); if (d->dir != d->direct_alloc_dir) free (d->dir); errno = ENOMEM; return -1; } #undef PRINTF_PARSE #undef DIRECTIVES #undef DIRECTIVE #undef CHAR_T_ONLY_ASCII #undef CHAR_T gnuastro-0.2.33-8a3b/bootstrapped/lib/printf-args.c0000644000175000017500000001463213004436754017005 00000000000000/* Decomposed printf argument list. Copyright (C) 1999, 2002-2003, 2005-2007, 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* This file can be parametrized with the following macros: ENABLE_UNISTDIO Set to 1 to enable the unistdio extensions. PRINTF_FETCHARGS Name of the function to be defined. STATIC Set to 'static' to declare the function static. */ #ifndef PRINTF_FETCHARGS # include #endif /* Specification. */ #ifndef PRINTF_FETCHARGS # include "printf-args.h" #endif #ifdef STATIC STATIC #endif int PRINTF_FETCHARGS (va_list args, arguments *a) { size_t i; argument *ap; for (i = 0, ap = &a->arg[0]; i < a->count; i++, ap++) switch (ap->type) { case TYPE_SCHAR: ap->a.a_schar = va_arg (args, /*signed char*/ int); break; case TYPE_UCHAR: ap->a.a_uchar = va_arg (args, /*unsigned char*/ int); break; case TYPE_SHORT: ap->a.a_short = va_arg (args, /*short*/ int); break; case TYPE_USHORT: ap->a.a_ushort = va_arg (args, /*unsigned short*/ int); break; case TYPE_INT: ap->a.a_int = va_arg (args, int); break; case TYPE_UINT: ap->a.a_uint = va_arg (args, unsigned int); break; case TYPE_LONGINT: ap->a.a_longint = va_arg (args, long int); break; case TYPE_ULONGINT: ap->a.a_ulongint = va_arg (args, unsigned long int); break; #if HAVE_LONG_LONG_INT case TYPE_LONGLONGINT: ap->a.a_longlongint = va_arg (args, long long int); break; case TYPE_ULONGLONGINT: ap->a.a_ulonglongint = va_arg (args, unsigned long long int); break; #endif case TYPE_DOUBLE: ap->a.a_double = va_arg (args, double); break; case TYPE_LONGDOUBLE: ap->a.a_longdouble = va_arg (args, long double); break; case TYPE_CHAR: ap->a.a_char = va_arg (args, int); break; #if HAVE_WINT_T case TYPE_WIDE_CHAR: /* Although ISO C 99 7.24.1.(2) says that wint_t is "unchanged by default argument promotions", this is not the case in mingw32, where wint_t is 'unsigned short'. */ ap->a.a_wide_char = (sizeof (wint_t) < sizeof (int) ? (wint_t) va_arg (args, int) : va_arg (args, wint_t)); break; #endif case TYPE_STRING: ap->a.a_string = va_arg (args, const char *); /* A null pointer is an invalid argument for "%s", but in practice it occurs quite frequently in printf statements that produce debug output. Use a fallback in this case. */ if (ap->a.a_string == NULL) ap->a.a_string = "(NULL)"; break; #if HAVE_WCHAR_T case TYPE_WIDE_STRING: ap->a.a_wide_string = va_arg (args, const wchar_t *); /* A null pointer is an invalid argument for "%ls", but in practice it occurs quite frequently in printf statements that produce debug output. Use a fallback in this case. */ if (ap->a.a_wide_string == NULL) { static const wchar_t wide_null_string[] = { (wchar_t)'(', (wchar_t)'N', (wchar_t)'U', (wchar_t)'L', (wchar_t)'L', (wchar_t)')', (wchar_t)0 }; ap->a.a_wide_string = wide_null_string; } break; #endif case TYPE_POINTER: ap->a.a_pointer = va_arg (args, void *); break; case TYPE_COUNT_SCHAR_POINTER: ap->a.a_count_schar_pointer = va_arg (args, signed char *); break; case TYPE_COUNT_SHORT_POINTER: ap->a.a_count_short_pointer = va_arg (args, short *); break; case TYPE_COUNT_INT_POINTER: ap->a.a_count_int_pointer = va_arg (args, int *); break; case TYPE_COUNT_LONGINT_POINTER: ap->a.a_count_longint_pointer = va_arg (args, long int *); break; #if HAVE_LONG_LONG_INT case TYPE_COUNT_LONGLONGINT_POINTER: ap->a.a_count_longlongint_pointer = va_arg (args, long long int *); break; #endif #if ENABLE_UNISTDIO /* The unistdio extensions. */ case TYPE_U8_STRING: ap->a.a_u8_string = va_arg (args, const uint8_t *); /* A null pointer is an invalid argument for "%U", but in practice it occurs quite frequently in printf statements that produce debug output. Use a fallback in this case. */ if (ap->a.a_u8_string == NULL) { static const uint8_t u8_null_string[] = { '(', 'N', 'U', 'L', 'L', ')', 0 }; ap->a.a_u8_string = u8_null_string; } break; case TYPE_U16_STRING: ap->a.a_u16_string = va_arg (args, const uint16_t *); /* A null pointer is an invalid argument for "%lU", but in practice it occurs quite frequently in printf statements that produce debug output. Use a fallback in this case. */ if (ap->a.a_u16_string == NULL) { static const uint16_t u16_null_string[] = { '(', 'N', 'U', 'L', 'L', ')', 0 }; ap->a.a_u16_string = u16_null_string; } break; case TYPE_U32_STRING: ap->a.a_u32_string = va_arg (args, const uint32_t *); /* A null pointer is an invalid argument for "%llU", but in practice it occurs quite frequently in printf statements that produce debug output. Use a fallback in this case. */ if (ap->a.a_u32_string == NULL) { static const uint32_t u32_null_string[] = { '(', 'N', 'U', 'L', 'L', ')', 0 }; ap->a.a_u32_string = u32_null_string; } break; #endif default: /* Unknown type. */ return -1; } return 0; } gnuastro-0.2.33-8a3b/bootstrapped/lib/asnprintf.c0000644000175000017500000000204613004436754016551 00000000000000/* Formatted output to strings. Copyright (C) 1999, 2002, 2006, 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include "vasnprintf.h" #include char * asnprintf (char *resultbuf, size_t *lengthp, const char *format, ...) { va_list args; char *result; va_start (args, format); result = vasnprintf (resultbuf, lengthp, format, args); va_end (args); return result; } gnuastro-0.2.33-8a3b/bootstrapped/lib/strnlen.c0000644000175000017500000000216413004436754016233 00000000000000/* Find the length of STRING, but scan at most MAXLEN characters. Copyright (C) 2005-2007, 2009-2016 Free Software Foundation, Inc. Written by Simon Josefsson. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include /* Find the length of STRING, but scan at most MAXLEN characters. If no '\0' terminator is found in that many characters, return MAXLEN. */ size_t strnlen (const char *string, size_t maxlen) { const char *end = memchr (string, '\0', maxlen); return end ? (size_t) (end - string) : maxlen; } gnuastro-0.2.33-8a3b/bootstrapped/lib/strndup.c0000644000175000017500000000202413004436754016240 00000000000000/* A replacement function, for systems that lack strndup. Copyright (C) 1996-1998, 2001-2003, 2005-2007, 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include #include char * strndup (char const *s, size_t n) { size_t len = strnlen (s, n); char *new = malloc (len + 1); if (new == NULL) return NULL; new[len] = '\0'; return memcpy (new, s, len); } gnuastro-0.2.33-8a3b/bootstrapped/lib/strerror-override.c0000644000175000017500000002146513004436754020252 00000000000000/* strerror-override.c --- POSIX compatible system error routine Copyright (C) 2010-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2010. */ #include #include "strerror-override.h" #include #if GNULIB_defined_EWINSOCK /* native Windows platforms */ # if HAVE_WINSOCK2_H # include # endif #endif /* If ERRNUM maps to an errno value defined by gnulib, return a string describing the error. Otherwise return NULL. */ const char * strerror_override (int errnum) { /* These error messages are taken from glibc/sysdeps/gnu/errlist.c. */ switch (errnum) { #if REPLACE_STRERROR_0 case 0: return "Success"; #endif #if GNULIB_defined_ESOCK /* native Windows platforms with older */ case EINPROGRESS: return "Operation now in progress"; case EALREADY: return "Operation already in progress"; case ENOTSOCK: return "Socket operation on non-socket"; case EDESTADDRREQ: return "Destination address required"; case EMSGSIZE: return "Message too long"; case EPROTOTYPE: return "Protocol wrong type for socket"; case ENOPROTOOPT: return "Protocol not available"; case EPROTONOSUPPORT: return "Protocol not supported"; case EOPNOTSUPP: return "Operation not supported"; case EAFNOSUPPORT: return "Address family not supported by protocol"; case EADDRINUSE: return "Address already in use"; case EADDRNOTAVAIL: return "Cannot assign requested address"; case ENETDOWN: return "Network is down"; case ENETUNREACH: return "Network is unreachable"; case ECONNRESET: return "Connection reset by peer"; case ENOBUFS: return "No buffer space available"; case EISCONN: return "Transport endpoint is already connected"; case ENOTCONN: return "Transport endpoint is not connected"; case ETIMEDOUT: return "Connection timed out"; case ECONNREFUSED: return "Connection refused"; case ELOOP: return "Too many levels of symbolic links"; case EHOSTUNREACH: return "No route to host"; case EWOULDBLOCK: return "Operation would block"; #endif #if GNULIB_defined_ESTREAMS /* native Windows platforms with older */ case ETXTBSY: return "Text file busy"; case ENODATA: return "No data available"; case ENOSR: return "Out of streams resources"; case ENOSTR: return "Device not a stream"; case ETIME: return "Timer expired"; case EOTHER: return "Other error"; #endif #if GNULIB_defined_EWINSOCK /* native Windows platforms */ case ESOCKTNOSUPPORT: return "Socket type not supported"; case EPFNOSUPPORT: return "Protocol family not supported"; case ESHUTDOWN: return "Cannot send after transport endpoint shutdown"; case ETOOMANYREFS: return "Too many references: cannot splice"; case EHOSTDOWN: return "Host is down"; case EPROCLIM: return "Too many processes"; case EUSERS: return "Too many users"; case EDQUOT: return "Disk quota exceeded"; case ESTALE: return "Stale NFS file handle"; case EREMOTE: return "Object is remote"; # if HAVE_WINSOCK2_H /* WSA_INVALID_HANDLE maps to EBADF */ /* WSA_NOT_ENOUGH_MEMORY maps to ENOMEM */ /* WSA_INVALID_PARAMETER maps to EINVAL */ case WSA_OPERATION_ABORTED: return "Overlapped operation aborted"; case WSA_IO_INCOMPLETE: return "Overlapped I/O event object not in signaled state"; case WSA_IO_PENDING: return "Overlapped operations will complete later"; /* WSAEINTR maps to EINTR */ /* WSAEBADF maps to EBADF */ /* WSAEACCES maps to EACCES */ /* WSAEFAULT maps to EFAULT */ /* WSAEINVAL maps to EINVAL */ /* WSAEMFILE maps to EMFILE */ /* WSAEWOULDBLOCK maps to EWOULDBLOCK */ /* WSAEINPROGRESS maps to EINPROGRESS */ /* WSAEALREADY maps to EALREADY */ /* WSAENOTSOCK maps to ENOTSOCK */ /* WSAEDESTADDRREQ maps to EDESTADDRREQ */ /* WSAEMSGSIZE maps to EMSGSIZE */ /* WSAEPROTOTYPE maps to EPROTOTYPE */ /* WSAENOPROTOOPT maps to ENOPROTOOPT */ /* WSAEPROTONOSUPPORT maps to EPROTONOSUPPORT */ /* WSAESOCKTNOSUPPORT is ESOCKTNOSUPPORT */ /* WSAEOPNOTSUPP maps to EOPNOTSUPP */ /* WSAEPFNOSUPPORT is EPFNOSUPPORT */ /* WSAEAFNOSUPPORT maps to EAFNOSUPPORT */ /* WSAEADDRINUSE maps to EADDRINUSE */ /* WSAEADDRNOTAVAIL maps to EADDRNOTAVAIL */ /* WSAENETDOWN maps to ENETDOWN */ /* WSAENETUNREACH maps to ENETUNREACH */ /* WSAENETRESET maps to ENETRESET */ /* WSAECONNABORTED maps to ECONNABORTED */ /* WSAECONNRESET maps to ECONNRESET */ /* WSAENOBUFS maps to ENOBUFS */ /* WSAEISCONN maps to EISCONN */ /* WSAENOTCONN maps to ENOTCONN */ /* WSAESHUTDOWN is ESHUTDOWN */ /* WSAETOOMANYREFS is ETOOMANYREFS */ /* WSAETIMEDOUT maps to ETIMEDOUT */ /* WSAECONNREFUSED maps to ECONNREFUSED */ /* WSAELOOP maps to ELOOP */ /* WSAENAMETOOLONG maps to ENAMETOOLONG */ /* WSAEHOSTDOWN is EHOSTDOWN */ /* WSAEHOSTUNREACH maps to EHOSTUNREACH */ /* WSAENOTEMPTY maps to ENOTEMPTY */ /* WSAEPROCLIM is EPROCLIM */ /* WSAEUSERS is EUSERS */ /* WSAEDQUOT is EDQUOT */ /* WSAESTALE is ESTALE */ /* WSAEREMOTE is EREMOTE */ case WSASYSNOTREADY: return "Network subsystem is unavailable"; case WSAVERNOTSUPPORTED: return "Winsock.dll version out of range"; case WSANOTINITIALISED: return "Successful WSAStartup not yet performed"; case WSAEDISCON: return "Graceful shutdown in progress"; case WSAENOMORE: case WSA_E_NO_MORE: return "No more results"; case WSAECANCELLED: case WSA_E_CANCELLED: return "Call was canceled"; case WSAEINVALIDPROCTABLE: return "Procedure call table is invalid"; case WSAEINVALIDPROVIDER: return "Service provider is invalid"; case WSAEPROVIDERFAILEDINIT: return "Service provider failed to initialize"; case WSASYSCALLFAILURE: return "System call failure"; case WSASERVICE_NOT_FOUND: return "Service not found"; case WSATYPE_NOT_FOUND: return "Class type not found"; case WSAEREFUSED: return "Database query was refused"; case WSAHOST_NOT_FOUND: return "Host not found"; case WSATRY_AGAIN: return "Nonauthoritative host not found"; case WSANO_RECOVERY: return "Nonrecoverable error"; case WSANO_DATA: return "Valid name, no data record of requested type"; /* WSA_QOS_* omitted */ # endif #endif #if GNULIB_defined_ENOMSG case ENOMSG: return "No message of desired type"; #endif #if GNULIB_defined_EIDRM case EIDRM: return "Identifier removed"; #endif #if GNULIB_defined_ENOLINK case ENOLINK: return "Link has been severed"; #endif #if GNULIB_defined_EPROTO case EPROTO: return "Protocol error"; #endif #if GNULIB_defined_EMULTIHOP case EMULTIHOP: return "Multihop attempted"; #endif #if GNULIB_defined_EBADMSG case EBADMSG: return "Bad message"; #endif #if GNULIB_defined_EOVERFLOW case EOVERFLOW: return "Value too large for defined data type"; #endif #if GNULIB_defined_ENOTSUP case ENOTSUP: return "Not supported"; #endif #if GNULIB_defined_ENETRESET case ENETRESET: return "Network dropped connection on reset"; #endif #if GNULIB_defined_ECONNABORTED case ECONNABORTED: return "Software caused connection abort"; #endif #if GNULIB_defined_ESTALE case ESTALE: return "Stale NFS file handle"; #endif #if GNULIB_defined_EDQUOT case EDQUOT: return "Disk quota exceeded"; #endif #if GNULIB_defined_ECANCELED case ECANCELED: return "Operation canceled"; #endif #if GNULIB_defined_EOWNERDEAD case EOWNERDEAD: return "Owner died"; #endif #if GNULIB_defined_ENOTRECOVERABLE case ENOTRECOVERABLE: return "State not recoverable"; #endif #if GNULIB_defined_EILSEQ case EILSEQ: return "Invalid or incomplete multibyte or wide character"; #endif default: return NULL; } } gnuastro-0.2.33-8a3b/bootstrapped/lib/strerror.c0000644000175000017500000000404313004436754016426 00000000000000/* strerror.c --- POSIX compatible system error routine Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include #include #include #include "intprops.h" #include "strerror-override.h" #include "verify.h" /* Use the system functions, not the gnulib overrides in this file. */ #undef sprintf char * strerror (int n) #undef strerror { static char buf[STACKBUF_LEN]; size_t len; /* Cast away const, due to the historical signature of strerror; callers should not be modifying the string. */ const char *msg = strerror_override (n); if (msg) return (char *) msg; msg = strerror (n); /* Our strerror_r implementation might use the system's strerror buffer, so all other clients of strerror have to see the error copied into a buffer that we manage. This is not thread-safe, even if the system strerror is, but portable programs shouldn't be using strerror if they care about thread-safety. */ if (!msg || !*msg) { static char const fmt[] = "Unknown error %d"; verify (sizeof buf >= sizeof (fmt) + INT_STRLEN_BOUND (n)); sprintf (buf, fmt, n); errno = EINVAL; return buf; } /* Fix STACKBUF_LEN if this ever aborts. */ len = strlen (msg); if (sizeof buf <= len) abort (); return memcpy (buf, msg, len + 1); } gnuastro-0.2.33-8a3b/bootstrapped/lib/strchrnul.c0000644000175000017500000001301513004436754016567 00000000000000/* Searching in a string. Copyright (C) 2003, 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include /* Find the first occurrence of C in S or the final NUL byte. */ char * strchrnul (const char *s, int c_in) { /* On 32-bit hardware, choosing longword to be a 32-bit unsigned long instead of a 64-bit uintmax_t tends to give better performance. On 64-bit hardware, unsigned long is generally 64 bits already. Change this typedef to experiment with performance. */ typedef unsigned long int longword; const unsigned char *char_ptr; const longword *longword_ptr; longword repeated_one; longword repeated_c; unsigned char c; c = (unsigned char) c_in; if (!c) return rawmemchr (s, 0); /* Handle the first few bytes by reading one byte at a time. Do this until CHAR_PTR is aligned on a longword boundary. */ for (char_ptr = (const unsigned char *) s; (size_t) char_ptr % sizeof (longword) != 0; ++char_ptr) if (!*char_ptr || *char_ptr == c) return (char *) char_ptr; longword_ptr = (const longword *) char_ptr; /* All these elucidatory comments refer to 4-byte longwords, but the theory applies equally well to any size longwords. */ /* Compute auxiliary longword values: repeated_one is a value which has a 1 in every byte. repeated_c has c in every byte. */ repeated_one = 0x01010101; repeated_c = c | (c << 8); repeated_c |= repeated_c << 16; if (0xffffffffU < (longword) -1) { repeated_one |= repeated_one << 31 << 1; repeated_c |= repeated_c << 31 << 1; if (8 < sizeof (longword)) { size_t i; for (i = 64; i < sizeof (longword) * 8; i *= 2) { repeated_one |= repeated_one << i; repeated_c |= repeated_c << i; } } } /* Instead of the traditional loop which tests each byte, we will test a longword at a time. The tricky part is testing if *any of the four* bytes in the longword in question are equal to NUL or c. We first use an xor with repeated_c. This reduces the task to testing whether *any of the four* bytes in longword1 or longword2 is zero. Let's consider longword1. We compute tmp = ((longword1 - repeated_one) & ~longword1) & (repeated_one << 7). That is, we perform the following operations: 1. Subtract repeated_one. 2. & ~longword1. 3. & a mask consisting of 0x80 in every byte. Consider what happens in each byte: - If a byte of longword1 is zero, step 1 and 2 transform it into 0xff, and step 3 transforms it into 0x80. A carry can also be propagated to more significant bytes. - If a byte of longword1 is nonzero, let its lowest 1 bit be at position k (0 <= k <= 7); so the lowest k bits are 0. After step 1, the byte ends in a single bit of value 0 and k bits of value 1. After step 2, the result is just k bits of value 1: 2^k - 1. After step 3, the result is 0. And no carry is produced. So, if longword1 has only non-zero bytes, tmp is zero. Whereas if longword1 has a zero byte, call j the position of the least significant zero byte. Then the result has a zero at positions 0, ..., j-1 and a 0x80 at position j. We cannot predict the result at the more significant bytes (positions j+1..3), but it does not matter since we already have a non-zero bit at position 8*j+7. The test whether any byte in longword1 or longword2 is zero is equivalent to testing whether tmp1 is nonzero or tmp2 is nonzero. We can combine this into a single test, whether (tmp1 | tmp2) is nonzero. This test can read more than one byte beyond the end of a string, depending on where the terminating NUL is encountered. However, this is considered safe since the initialization phase ensured that the read will be aligned, therefore, the read will not cross page boundaries and will not cause a fault. */ while (1) { longword longword1 = *longword_ptr ^ repeated_c; longword longword2 = *longword_ptr; if (((((longword1 - repeated_one) & ~longword1) | ((longword2 - repeated_one) & ~longword2)) & (repeated_one << 7)) != 0) break; longword_ptr++; } char_ptr = (const unsigned char *) longword_ptr; /* At this point, we know that one of the sizeof (longword) bytes starting at char_ptr is == 0 or == c. On little-endian machines, we could determine the first such byte without any further memory accesses, just by looking at the tmp result from the last loop iteration. But this does not work on big-endian machines. Choose code that works in both cases. */ char_ptr = (unsigned char *) longword_ptr; while (*char_ptr && (*char_ptr != c)) char_ptr++; return (char *) char_ptr; } gnuastro-0.2.33-8a3b/bootstrapped/lib/strncasecmp.c0000644000175000017500000000355713004436754017077 00000000000000/* strncasecmp.c -- case insensitive string comparator Copyright (C) 1998-1999, 2005-2007, 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include #include #include #define TOLOWER(Ch) (isupper (Ch) ? tolower (Ch) : (Ch)) /* Compare no more than N bytes of strings S1 and S2, ignoring case, returning less than, equal to or greater than zero if S1 is lexicographically less than, equal to or greater than S2. Note: This function cannot work correctly in multibyte locales. */ int strncasecmp (const char *s1, const char *s2, size_t n) { register const unsigned char *p1 = (const unsigned char *) s1; register const unsigned char *p2 = (const unsigned char *) s2; unsigned char c1, c2; if (p1 == p2 || n == 0) return 0; do { c1 = TOLOWER (*p1); c2 = TOLOWER (*p2); if (--n == 0 || c1 == '\0') break; ++p1; ++p2; } while (c1 == c2); if (UCHAR_MAX <= INT_MAX) return c1 - c2; else /* On machines where 'char' and 'int' are types of the same size, the difference of two 'unsigned char' values - including the sign bit - doesn't fit in an 'int'. */ return (c1 > c2 ? 1 : c1 < c2 ? -1 : 0); } gnuastro-0.2.33-8a3b/bootstrapped/lib/strcasecmp.c0000644000175000017500000000342713004436754016715 00000000000000/* Case-insensitive string comparison function. Copyright (C) 1998-1999, 2005-2007, 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include #include #include #define TOLOWER(Ch) (isupper (Ch) ? tolower (Ch) : (Ch)) /* Compare strings S1 and S2, ignoring case, returning less than, equal to or greater than zero if S1 is lexicographically less than, equal to or greater than S2. Note: This function does not work with multibyte strings! */ int strcasecmp (const char *s1, const char *s2) { const unsigned char *p1 = (const unsigned char *) s1; const unsigned char *p2 = (const unsigned char *) s2; unsigned char c1, c2; if (p1 == p2) return 0; do { c1 = TOLOWER (*p1); c2 = TOLOWER (*p2); if (c1 == '\0') break; ++p1; ++p2; } while (c1 == c2); if (UCHAR_MAX <= INT_MAX) return c1 - c2; else /* On machines where 'char' and 'int' are types of the same size, the difference of two 'unsigned char' values - including the sign bit - doesn't fit in an 'int'. */ return (c1 > c2 ? 1 : c1 < c2 ? -1 : 0); } gnuastro-0.2.33-8a3b/bootstrapped/lib/sleep.c0000644000175000017500000000440713004436754015660 00000000000000/* Pausing execution of the current thread. Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2007. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include "verify.h" #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # define WIN32_LEAN_AND_MEAN /* avoid including junk */ # include unsigned int sleep (unsigned int seconds) { unsigned int remaining; /* Sleep for 1 second many times, because 1. Sleep is not interruptible by Ctrl-C, 2. we want to avoid arithmetic overflow while multiplying with 1000. */ for (remaining = seconds; remaining > 0; remaining--) Sleep (1000); return remaining; } #elif HAVE_SLEEP # undef sleep /* Guarantee unlimited sleep and a reasonable return value. Cygwin 1.5.x rejects attempts to sleep more than 49.7 days (2**32 milliseconds), but uses uninitialized memory which results in a garbage answer. Similarly, Linux 2.6.9 with glibc 2.3.4 has a too small return value when asked to sleep more than 24.85 days. */ unsigned int rpl_sleep (unsigned int seconds) { /* This requires int larger than 16 bits. */ verify (UINT_MAX / 24 / 24 / 60 / 60); const unsigned int limit = 24 * 24 * 60 * 60; while (limit < seconds) { unsigned int result; seconds -= limit; result = sleep (limit); if (result) return seconds + result; } return sleep (seconds); } #else /* !HAVE_SLEEP */ #error "Please port gnulib sleep.c to your platform, possibly using usleep() or select(), then report this to bug-gnulib." #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/regexec.c0000644000175000017500000037642113004436754016202 00000000000000/* Extended regular expression matching and search library. Copyright (C) 2002-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Contributed by Isamu Hasegawa . The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ static reg_errcode_t match_ctx_init (re_match_context_t *cache, int eflags, Idx n) internal_function; static void match_ctx_clean (re_match_context_t *mctx) internal_function; static void match_ctx_free (re_match_context_t *cache) internal_function; static reg_errcode_t match_ctx_add_entry (re_match_context_t *cache, Idx node, Idx str_idx, Idx from, Idx to) internal_function; static Idx search_cur_bkref_entry (const re_match_context_t *mctx, Idx str_idx) internal_function; static reg_errcode_t match_ctx_add_subtop (re_match_context_t *mctx, Idx node, Idx str_idx) internal_function; static re_sub_match_last_t * match_ctx_add_sublast (re_sub_match_top_t *subtop, Idx node, Idx str_idx) internal_function; static void sift_ctx_init (re_sift_context_t *sctx, re_dfastate_t **sifted_sts, re_dfastate_t **limited_sts, Idx last_node, Idx last_str_idx) internal_function; static reg_errcode_t re_search_internal (const regex_t *preg, const char *string, Idx length, Idx start, Idx last_start, Idx stop, size_t nmatch, regmatch_t pmatch[], int eflags) internal_function; static regoff_t re_search_2_stub (struct re_pattern_buffer *bufp, const char *string1, Idx length1, const char *string2, Idx length2, Idx start, regoff_t range, struct re_registers *regs, Idx stop, bool ret_len) internal_function; static regoff_t re_search_stub (struct re_pattern_buffer *bufp, const char *string, Idx length, Idx start, regoff_t range, Idx stop, struct re_registers *regs, bool ret_len) internal_function; static unsigned re_copy_regs (struct re_registers *regs, regmatch_t *pmatch, Idx nregs, int regs_allocated) internal_function; static reg_errcode_t prune_impossible_nodes (re_match_context_t *mctx) internal_function; static Idx check_matching (re_match_context_t *mctx, bool fl_longest_match, Idx *p_match_first) internal_function; static Idx check_halt_state_context (const re_match_context_t *mctx, const re_dfastate_t *state, Idx idx) internal_function; static void update_regs (const re_dfa_t *dfa, regmatch_t *pmatch, regmatch_t *prev_idx_match, Idx cur_node, Idx cur_idx, Idx nmatch) internal_function; static reg_errcode_t push_fail_stack (struct re_fail_stack_t *fs, Idx str_idx, Idx dest_node, Idx nregs, regmatch_t *regs, re_node_set *eps_via_nodes) internal_function; static reg_errcode_t set_regs (const regex_t *preg, const re_match_context_t *mctx, size_t nmatch, regmatch_t *pmatch, bool fl_backtrack) internal_function; static reg_errcode_t free_fail_stack_return (struct re_fail_stack_t *fs) internal_function; #ifdef RE_ENABLE_I18N static int sift_states_iter_mb (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx node_idx, Idx str_idx, Idx max_str_idx) internal_function; #endif /* RE_ENABLE_I18N */ static reg_errcode_t sift_states_backward (const re_match_context_t *mctx, re_sift_context_t *sctx) internal_function; static reg_errcode_t build_sifted_states (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx str_idx, re_node_set *cur_dest) internal_function; static reg_errcode_t update_cur_sifted_state (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx str_idx, re_node_set *dest_nodes) internal_function; static reg_errcode_t add_epsilon_src_nodes (const re_dfa_t *dfa, re_node_set *dest_nodes, const re_node_set *candidates) internal_function; static bool check_dst_limits (const re_match_context_t *mctx, const re_node_set *limits, Idx dst_node, Idx dst_idx, Idx src_node, Idx src_idx) internal_function; static int check_dst_limits_calc_pos_1 (const re_match_context_t *mctx, int boundaries, Idx subexp_idx, Idx from_node, Idx bkref_idx) internal_function; static int check_dst_limits_calc_pos (const re_match_context_t *mctx, Idx limit, Idx subexp_idx, Idx node, Idx str_idx, Idx bkref_idx) internal_function; static reg_errcode_t check_subexp_limits (const re_dfa_t *dfa, re_node_set *dest_nodes, const re_node_set *candidates, re_node_set *limits, struct re_backref_cache_entry *bkref_ents, Idx str_idx) internal_function; static reg_errcode_t sift_states_bkref (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx str_idx, const re_node_set *candidates) internal_function; static reg_errcode_t merge_state_array (const re_dfa_t *dfa, re_dfastate_t **dst, re_dfastate_t **src, Idx num) internal_function; static re_dfastate_t *find_recover_state (reg_errcode_t *err, re_match_context_t *mctx) internal_function; static re_dfastate_t *transit_state (reg_errcode_t *err, re_match_context_t *mctx, re_dfastate_t *state) internal_function; static re_dfastate_t *merge_state_with_log (reg_errcode_t *err, re_match_context_t *mctx, re_dfastate_t *next_state) internal_function; static reg_errcode_t check_subexp_matching_top (re_match_context_t *mctx, re_node_set *cur_nodes, Idx str_idx) internal_function; #if 0 static re_dfastate_t *transit_state_sb (reg_errcode_t *err, re_match_context_t *mctx, re_dfastate_t *pstate) internal_function; #endif #ifdef RE_ENABLE_I18N static reg_errcode_t transit_state_mb (re_match_context_t *mctx, re_dfastate_t *pstate) internal_function; #endif /* RE_ENABLE_I18N */ static reg_errcode_t transit_state_bkref (re_match_context_t *mctx, const re_node_set *nodes) internal_function; static reg_errcode_t get_subexp (re_match_context_t *mctx, Idx bkref_node, Idx bkref_str_idx) internal_function; static reg_errcode_t get_subexp_sub (re_match_context_t *mctx, const re_sub_match_top_t *sub_top, re_sub_match_last_t *sub_last, Idx bkref_node, Idx bkref_str) internal_function; static Idx find_subexp_node (const re_dfa_t *dfa, const re_node_set *nodes, Idx subexp_idx, int type) internal_function; static reg_errcode_t check_arrival (re_match_context_t *mctx, state_array_t *path, Idx top_node, Idx top_str, Idx last_node, Idx last_str, int type) internal_function; static reg_errcode_t check_arrival_add_next_nodes (re_match_context_t *mctx, Idx str_idx, re_node_set *cur_nodes, re_node_set *next_nodes) internal_function; static reg_errcode_t check_arrival_expand_ecl (const re_dfa_t *dfa, re_node_set *cur_nodes, Idx ex_subexp, int type) internal_function; static reg_errcode_t check_arrival_expand_ecl_sub (const re_dfa_t *dfa, re_node_set *dst_nodes, Idx target, Idx ex_subexp, int type) internal_function; static reg_errcode_t expand_bkref_cache (re_match_context_t *mctx, re_node_set *cur_nodes, Idx cur_str, Idx subexp_num, int type) internal_function; static bool build_trtable (const re_dfa_t *dfa, re_dfastate_t *state) internal_function; #ifdef RE_ENABLE_I18N static int check_node_accept_bytes (const re_dfa_t *dfa, Idx node_idx, const re_string_t *input, Idx idx) internal_function; # ifdef _LIBC static unsigned int find_collation_sequence_value (const unsigned char *mbs, size_t name_len) internal_function; # endif /* _LIBC */ #endif /* RE_ENABLE_I18N */ static Idx group_nodes_into_DFAstates (const re_dfa_t *dfa, const re_dfastate_t *state, re_node_set *states_node, bitset_t *states_ch) internal_function; static bool check_node_accept (const re_match_context_t *mctx, const re_token_t *node, Idx idx) internal_function; static reg_errcode_t extend_buffers (re_match_context_t *mctx, int min_len) internal_function; /* Entry point for POSIX code. */ /* regexec searches for a given pattern, specified by PREG, in the string STRING. If NMATCH is zero or REG_NOSUB was set in the cflags argument to 'regcomp', we ignore PMATCH. Otherwise, we assume PMATCH has at least NMATCH elements, and we set them to the offsets of the corresponding matched substrings. EFLAGS specifies "execution flags" which affect matching: if REG_NOTBOL is set, then ^ does not match at the beginning of the string; if REG_NOTEOL is set, then $ does not match at the end. We return 0 if we find a match and REG_NOMATCH if not. */ int regexec (const regex_t *_Restrict_ preg, const char *_Restrict_ string, size_t nmatch, regmatch_t pmatch[], int eflags) { reg_errcode_t err; Idx start, length; re_dfa_t *dfa = preg->buffer; if (eflags & ~(REG_NOTBOL | REG_NOTEOL | REG_STARTEND)) return REG_BADPAT; if (eflags & REG_STARTEND) { start = pmatch[0].rm_so; length = pmatch[0].rm_eo; } else { start = 0; length = strlen (string); } lock_lock (dfa->lock); if (preg->no_sub) err = re_search_internal (preg, string, length, start, length, length, 0, NULL, eflags); else err = re_search_internal (preg, string, length, start, length, length, nmatch, pmatch, eflags); lock_unlock (dfa->lock); return err != REG_NOERROR; } #ifdef _LIBC # include versioned_symbol (libc, __regexec, regexec, GLIBC_2_3_4); # if SHLIB_COMPAT (libc, GLIBC_2_0, GLIBC_2_3_4) __typeof__ (__regexec) __compat_regexec; int attribute_compat_text_section __compat_regexec (const regex_t *_Restrict_ preg, const char *_Restrict_ string, size_t nmatch, regmatch_t pmatch[], int eflags) { return regexec (preg, string, nmatch, pmatch, eflags & (REG_NOTBOL | REG_NOTEOL)); } compat_symbol (libc, __compat_regexec, regexec, GLIBC_2_0); # endif #endif /* Entry points for GNU code. */ /* re_match, re_search, re_match_2, re_search_2 The former two functions operate on STRING with length LENGTH, while the later two operate on concatenation of STRING1 and STRING2 with lengths LENGTH1 and LENGTH2, respectively. re_match() matches the compiled pattern in BUFP against the string, starting at index START. re_search() first tries matching at index START, then it tries to match starting from index START + 1, and so on. The last start position tried is START + RANGE. (Thus RANGE = 0 forces re_search to operate the same way as re_match().) The parameter STOP of re_{match,search}_2 specifies that no match exceeding the first STOP characters of the concatenation of the strings should be concerned. If REGS is not NULL, and BUFP->no_sub is not set, the offsets of the match and all groups is stored in REGS. (For the "_2" variants, the offsets are computed relative to the concatenation, not relative to the individual strings.) On success, re_match* functions return the length of the match, re_search* return the position of the start of the match. Return value -1 means no match was found and -2 indicates an internal error. */ regoff_t re_match (struct re_pattern_buffer *bufp, const char *string, Idx length, Idx start, struct re_registers *regs) { return re_search_stub (bufp, string, length, start, 0, length, regs, true); } #ifdef _LIBC weak_alias (__re_match, re_match) #endif regoff_t re_search (struct re_pattern_buffer *bufp, const char *string, Idx length, Idx start, regoff_t range, struct re_registers *regs) { return re_search_stub (bufp, string, length, start, range, length, regs, false); } #ifdef _LIBC weak_alias (__re_search, re_search) #endif regoff_t re_match_2 (struct re_pattern_buffer *bufp, const char *string1, Idx length1, const char *string2, Idx length2, Idx start, struct re_registers *regs, Idx stop) { return re_search_2_stub (bufp, string1, length1, string2, length2, start, 0, regs, stop, true); } #ifdef _LIBC weak_alias (__re_match_2, re_match_2) #endif regoff_t re_search_2 (struct re_pattern_buffer *bufp, const char *string1, Idx length1, const char *string2, Idx length2, Idx start, regoff_t range, struct re_registers *regs, Idx stop) { return re_search_2_stub (bufp, string1, length1, string2, length2, start, range, regs, stop, false); } #ifdef _LIBC weak_alias (__re_search_2, re_search_2) #endif static regoff_t internal_function re_search_2_stub (struct re_pattern_buffer *bufp, const char *string1, Idx length1, const char *string2, Idx length2, Idx start, regoff_t range, struct re_registers *regs, Idx stop, bool ret_len) { const char *str; regoff_t rval; Idx len = length1 + length2; char *s = NULL; if (BE (length1 < 0 || length2 < 0 || stop < 0 || len < length1, 0)) return -2; /* Concatenate the strings. */ if (length2 > 0) if (length1 > 0) { s = re_malloc (char, len); if (BE (s == NULL, 0)) return -2; #ifdef _LIBC memcpy (__mempcpy (s, string1, length1), string2, length2); #else memcpy (s, string1, length1); memcpy (s + length1, string2, length2); #endif str = s; } else str = string2; else str = string1; rval = re_search_stub (bufp, str, len, start, range, stop, regs, ret_len); re_free (s); return rval; } /* The parameters have the same meaning as those of re_search. Additional parameters: If RET_LEN is true the length of the match is returned (re_match style); otherwise the position of the match is returned. */ static regoff_t internal_function re_search_stub (struct re_pattern_buffer *bufp, const char *string, Idx length, Idx start, regoff_t range, Idx stop, struct re_registers *regs, bool ret_len) { reg_errcode_t result; regmatch_t *pmatch; Idx nregs; regoff_t rval; int eflags = 0; re_dfa_t *dfa = bufp->buffer; Idx last_start = start + range; /* Check for out-of-range. */ if (BE (start < 0 || start > length, 0)) return -1; if (BE (length < last_start || (0 <= range && last_start < start), 0)) last_start = length; else if (BE (last_start < 0 || (range < 0 && start <= last_start), 0)) last_start = 0; lock_lock (dfa->lock); eflags |= (bufp->not_bol) ? REG_NOTBOL : 0; eflags |= (bufp->not_eol) ? REG_NOTEOL : 0; /* Compile fastmap if we haven't yet. */ if (start < last_start && bufp->fastmap != NULL && !bufp->fastmap_accurate) re_compile_fastmap (bufp); if (BE (bufp->no_sub, 0)) regs = NULL; /* We need at least 1 register. */ if (regs == NULL) nregs = 1; else if (BE (bufp->regs_allocated == REGS_FIXED && regs->num_regs <= bufp->re_nsub, 0)) { nregs = regs->num_regs; if (BE (nregs < 1, 0)) { /* Nothing can be copied to regs. */ regs = NULL; nregs = 1; } } else nregs = bufp->re_nsub + 1; pmatch = re_malloc (regmatch_t, nregs); if (BE (pmatch == NULL, 0)) { rval = -2; goto out; } result = re_search_internal (bufp, string, length, start, last_start, stop, nregs, pmatch, eflags); rval = 0; /* I hope we needn't fill their regs with -1's when no match was found. */ if (result != REG_NOERROR) rval = result == REG_NOMATCH ? -1 : -2; else if (regs != NULL) { /* If caller wants register contents data back, copy them. */ bufp->regs_allocated = re_copy_regs (regs, pmatch, nregs, bufp->regs_allocated); if (BE (bufp->regs_allocated == REGS_UNALLOCATED, 0)) rval = -2; } if (BE (rval == 0, 1)) { if (ret_len) { assert (pmatch[0].rm_so == start); rval = pmatch[0].rm_eo - start; } else rval = pmatch[0].rm_so; } re_free (pmatch); out: lock_unlock (dfa->lock); return rval; } static unsigned internal_function re_copy_regs (struct re_registers *regs, regmatch_t *pmatch, Idx nregs, int regs_allocated) { int rval = REGS_REALLOCATE; Idx i; Idx need_regs = nregs + 1; /* We need one extra element beyond 'num_regs' for the '-1' marker GNU code uses. */ /* Have the register data arrays been allocated? */ if (regs_allocated == REGS_UNALLOCATED) { /* No. So allocate them with malloc. */ regs->start = re_malloc (regoff_t, need_regs); if (BE (regs->start == NULL, 0)) return REGS_UNALLOCATED; regs->end = re_malloc (regoff_t, need_regs); if (BE (regs->end == NULL, 0)) { re_free (regs->start); return REGS_UNALLOCATED; } regs->num_regs = need_regs; } else if (regs_allocated == REGS_REALLOCATE) { /* Yes. If we need more elements than were already allocated, reallocate them. If we need fewer, just leave it alone. */ if (BE (need_regs > regs->num_regs, 0)) { regoff_t *new_start = re_realloc (regs->start, regoff_t, need_regs); regoff_t *new_end; if (BE (new_start == NULL, 0)) return REGS_UNALLOCATED; new_end = re_realloc (regs->end, regoff_t, need_regs); if (BE (new_end == NULL, 0)) { re_free (new_start); return REGS_UNALLOCATED; } regs->start = new_start; regs->end = new_end; regs->num_regs = need_regs; } } else { assert (regs_allocated == REGS_FIXED); /* This function may not be called with REGS_FIXED and nregs too big. */ assert (regs->num_regs >= nregs); rval = REGS_FIXED; } /* Copy the regs. */ for (i = 0; i < nregs; ++i) { regs->start[i] = pmatch[i].rm_so; regs->end[i] = pmatch[i].rm_eo; } for ( ; i < regs->num_regs; ++i) regs->start[i] = regs->end[i] = -1; return rval; } /* Set REGS to hold NUM_REGS registers, storing them in STARTS and ENDS. Subsequent matches using PATTERN_BUFFER and REGS will use this memory for recording register information. STARTS and ENDS must be allocated using the malloc library routine, and must each be at least NUM_REGS * sizeof (regoff_t) bytes long. If NUM_REGS == 0, then subsequent matches should allocate their own register data. Unless this function is called, the first search or match using PATTERN_BUFFER will allocate its own register data, without freeing the old data. */ void re_set_registers (struct re_pattern_buffer *bufp, struct re_registers *regs, __re_size_t num_regs, regoff_t *starts, regoff_t *ends) { if (num_regs) { bufp->regs_allocated = REGS_REALLOCATE; regs->num_regs = num_regs; regs->start = starts; regs->end = ends; } else { bufp->regs_allocated = REGS_UNALLOCATED; regs->num_regs = 0; regs->start = regs->end = NULL; } } #ifdef _LIBC weak_alias (__re_set_registers, re_set_registers) #endif /* Entry points compatible with 4.2 BSD regex library. We don't define them unless specifically requested. */ #if defined _REGEX_RE_COMP || defined _LIBC int # ifdef _LIBC weak_function # endif re_exec (const char *s) { return 0 == regexec (&re_comp_buf, s, 0, NULL, 0); } #endif /* _REGEX_RE_COMP */ /* Internal entry point. */ /* Searches for a compiled pattern PREG in the string STRING, whose length is LENGTH. NMATCH, PMATCH, and EFLAGS have the same meaning as with regexec. LAST_START is START + RANGE, where START and RANGE have the same meaning as with re_search. Return REG_NOERROR if we find a match, and REG_NOMATCH if not, otherwise return the error code. Note: We assume front end functions already check ranges. (0 <= LAST_START && LAST_START <= LENGTH) */ static reg_errcode_t __attribute_warn_unused_result__ internal_function re_search_internal (const regex_t *preg, const char *string, Idx length, Idx start, Idx last_start, Idx stop, size_t nmatch, regmatch_t pmatch[], int eflags) { reg_errcode_t err; const re_dfa_t *dfa = preg->buffer; Idx left_lim, right_lim; int incr; bool fl_longest_match; int match_kind; Idx match_first; Idx match_last = -1; Idx extra_nmatch; bool sb; int ch; #if defined _LIBC || (defined __STDC_VERSION__ && __STDC_VERSION__ >= 199901L) re_match_context_t mctx = { .dfa = dfa }; #else re_match_context_t mctx; #endif char *fastmap = ((preg->fastmap != NULL && preg->fastmap_accurate && start != last_start && !preg->can_be_null) ? preg->fastmap : NULL); RE_TRANSLATE_TYPE t = preg->translate; #if !(defined _LIBC || (defined __STDC_VERSION__ && __STDC_VERSION__ >= 199901L)) memset (&mctx, '\0', sizeof (re_match_context_t)); mctx.dfa = dfa; #endif extra_nmatch = (nmatch > preg->re_nsub) ? nmatch - (preg->re_nsub + 1) : 0; nmatch -= extra_nmatch; /* Check if the DFA haven't been compiled. */ if (BE (preg->used == 0 || dfa->init_state == NULL || dfa->init_state_word == NULL || dfa->init_state_nl == NULL || dfa->init_state_begbuf == NULL, 0)) return REG_NOMATCH; #ifdef DEBUG /* We assume front-end functions already check them. */ assert (0 <= last_start && last_start <= length); #endif /* If initial states with non-begbuf contexts have no elements, the regex must be anchored. If preg->newline_anchor is set, we'll never use init_state_nl, so do not check it. */ if (dfa->init_state->nodes.nelem == 0 && dfa->init_state_word->nodes.nelem == 0 && (dfa->init_state_nl->nodes.nelem == 0 || !preg->newline_anchor)) { if (start != 0 && last_start != 0) return REG_NOMATCH; start = last_start = 0; } /* We must check the longest matching, if nmatch > 0. */ fl_longest_match = (nmatch != 0 || dfa->nbackref); err = re_string_allocate (&mctx.input, string, length, dfa->nodes_len + 1, preg->translate, (preg->syntax & RE_ICASE) != 0, dfa); if (BE (err != REG_NOERROR, 0)) goto free_return; mctx.input.stop = stop; mctx.input.raw_stop = stop; mctx.input.newline_anchor = preg->newline_anchor; err = match_ctx_init (&mctx, eflags, dfa->nbackref * 2); if (BE (err != REG_NOERROR, 0)) goto free_return; /* We will log all the DFA states through which the dfa pass, if nmatch > 1, or this dfa has "multibyte node", which is a back-reference or a node which can accept multibyte character or multi character collating element. */ if (nmatch > 1 || dfa->has_mb_node) { /* Avoid overflow. */ if (BE ((MIN (IDX_MAX, SIZE_MAX / sizeof (re_dfastate_t *)) <= mctx.input.bufs_len), 0)) { err = REG_ESPACE; goto free_return; } mctx.state_log = re_malloc (re_dfastate_t *, mctx.input.bufs_len + 1); if (BE (mctx.state_log == NULL, 0)) { err = REG_ESPACE; goto free_return; } } else mctx.state_log = NULL; match_first = start; mctx.input.tip_context = (eflags & REG_NOTBOL) ? CONTEXT_BEGBUF : CONTEXT_NEWLINE | CONTEXT_BEGBUF; /* Check incrementally whether the input string matches. */ incr = (last_start < start) ? -1 : 1; left_lim = (last_start < start) ? last_start : start; right_lim = (last_start < start) ? start : last_start; sb = dfa->mb_cur_max == 1; match_kind = (fastmap ? ((sb || !(preg->syntax & RE_ICASE || t) ? 4 : 0) | (start <= last_start ? 2 : 0) | (t != NULL ? 1 : 0)) : 8); for (;; match_first += incr) { err = REG_NOMATCH; if (match_first < left_lim || right_lim < match_first) goto free_return; /* Advance as rapidly as possible through the string, until we find a plausible place to start matching. This may be done with varying efficiency, so there are various possibilities: only the most common of them are specialized, in order to save on code size. We use a switch statement for speed. */ switch (match_kind) { case 8: /* No fastmap. */ break; case 7: /* Fastmap with single-byte translation, match forward. */ while (BE (match_first < right_lim, 1) && !fastmap[t[(unsigned char) string[match_first]]]) ++match_first; goto forward_match_found_start_or_reached_end; case 6: /* Fastmap without translation, match forward. */ while (BE (match_first < right_lim, 1) && !fastmap[(unsigned char) string[match_first]]) ++match_first; forward_match_found_start_or_reached_end: if (BE (match_first == right_lim, 0)) { ch = match_first >= length ? 0 : (unsigned char) string[match_first]; if (!fastmap[t ? t[ch] : ch]) goto free_return; } break; case 4: case 5: /* Fastmap without multi-byte translation, match backwards. */ while (match_first >= left_lim) { ch = match_first >= length ? 0 : (unsigned char) string[match_first]; if (fastmap[t ? t[ch] : ch]) break; --match_first; } if (match_first < left_lim) goto free_return; break; default: /* In this case, we can't determine easily the current byte, since it might be a component byte of a multibyte character. Then we use the constructed buffer instead. */ for (;;) { /* If MATCH_FIRST is out of the valid range, reconstruct the buffers. */ __re_size_t offset = match_first - mctx.input.raw_mbs_idx; if (BE (offset >= (__re_size_t) mctx.input.valid_raw_len, 0)) { err = re_string_reconstruct (&mctx.input, match_first, eflags); if (BE (err != REG_NOERROR, 0)) goto free_return; offset = match_first - mctx.input.raw_mbs_idx; } /* If MATCH_FIRST is out of the buffer, leave it as '\0'. Note that MATCH_FIRST must not be smaller than 0. */ ch = (match_first >= length ? 0 : re_string_byte_at (&mctx.input, offset)); if (fastmap[ch]) break; match_first += incr; if (match_first < left_lim || match_first > right_lim) { err = REG_NOMATCH; goto free_return; } } break; } /* Reconstruct the buffers so that the matcher can assume that the matching starts from the beginning of the buffer. */ err = re_string_reconstruct (&mctx.input, match_first, eflags); if (BE (err != REG_NOERROR, 0)) goto free_return; #ifdef RE_ENABLE_I18N /* Don't consider this char as a possible match start if it part, yet isn't the head, of a multibyte character. */ if (!sb && !re_string_first_byte (&mctx.input, 0)) continue; #endif /* It seems to be appropriate one, then use the matcher. */ /* We assume that the matching starts from 0. */ mctx.state_log_top = mctx.nbkref_ents = mctx.max_mb_elem_len = 0; match_last = check_matching (&mctx, fl_longest_match, start <= last_start ? &match_first : NULL); if (match_last != -1) { if (BE (match_last == -2, 0)) { err = REG_ESPACE; goto free_return; } else { mctx.match_last = match_last; if ((!preg->no_sub && nmatch > 1) || dfa->nbackref) { re_dfastate_t *pstate = mctx.state_log[match_last]; mctx.last_node = check_halt_state_context (&mctx, pstate, match_last); } if ((!preg->no_sub && nmatch > 1 && dfa->has_plural_match) || dfa->nbackref) { err = prune_impossible_nodes (&mctx); if (err == REG_NOERROR) break; if (BE (err != REG_NOMATCH, 0)) goto free_return; match_last = -1; } else break; /* We found a match. */ } } match_ctx_clean (&mctx); } #ifdef DEBUG assert (match_last != -1); assert (err == REG_NOERROR); #endif /* Set pmatch[] if we need. */ if (nmatch > 0) { Idx reg_idx; /* Initialize registers. */ for (reg_idx = 1; reg_idx < nmatch; ++reg_idx) pmatch[reg_idx].rm_so = pmatch[reg_idx].rm_eo = -1; /* Set the points where matching start/end. */ pmatch[0].rm_so = 0; pmatch[0].rm_eo = mctx.match_last; /* FIXME: This function should fail if mctx.match_last exceeds the maximum possible regoff_t value. We need a new error code REG_OVERFLOW. */ if (!preg->no_sub && nmatch > 1) { err = set_regs (preg, &mctx, nmatch, pmatch, dfa->has_plural_match && dfa->nbackref > 0); if (BE (err != REG_NOERROR, 0)) goto free_return; } /* At last, add the offset to each register, since we slid the buffers so that we could assume that the matching starts from 0. */ for (reg_idx = 0; reg_idx < nmatch; ++reg_idx) if (pmatch[reg_idx].rm_so != -1) { #ifdef RE_ENABLE_I18N if (BE (mctx.input.offsets_needed != 0, 0)) { pmatch[reg_idx].rm_so = (pmatch[reg_idx].rm_so == mctx.input.valid_len ? mctx.input.valid_raw_len : mctx.input.offsets[pmatch[reg_idx].rm_so]); pmatch[reg_idx].rm_eo = (pmatch[reg_idx].rm_eo == mctx.input.valid_len ? mctx.input.valid_raw_len : mctx.input.offsets[pmatch[reg_idx].rm_eo]); } #else assert (mctx.input.offsets_needed == 0); #endif pmatch[reg_idx].rm_so += match_first; pmatch[reg_idx].rm_eo += match_first; } for (reg_idx = 0; reg_idx < extra_nmatch; ++reg_idx) { pmatch[nmatch + reg_idx].rm_so = -1; pmatch[nmatch + reg_idx].rm_eo = -1; } if (dfa->subexp_map) for (reg_idx = 0; reg_idx + 1 < nmatch; reg_idx++) if (dfa->subexp_map[reg_idx] != reg_idx) { pmatch[reg_idx + 1].rm_so = pmatch[dfa->subexp_map[reg_idx] + 1].rm_so; pmatch[reg_idx + 1].rm_eo = pmatch[dfa->subexp_map[reg_idx] + 1].rm_eo; } } free_return: re_free (mctx.state_log); if (dfa->nbackref) match_ctx_free (&mctx); re_string_destruct (&mctx.input); return err; } static reg_errcode_t internal_function __attribute_warn_unused_result__ prune_impossible_nodes (re_match_context_t *mctx) { const re_dfa_t *const dfa = mctx->dfa; Idx halt_node, match_last; reg_errcode_t ret; re_dfastate_t **sifted_states; re_dfastate_t **lim_states = NULL; re_sift_context_t sctx; #ifdef DEBUG assert (mctx->state_log != NULL); #endif match_last = mctx->match_last; halt_node = mctx->last_node; /* Avoid overflow. */ if (BE (MIN (IDX_MAX, SIZE_MAX / sizeof (re_dfastate_t *)) <= match_last, 0)) return REG_ESPACE; sifted_states = re_malloc (re_dfastate_t *, match_last + 1); if (BE (sifted_states == NULL, 0)) { ret = REG_ESPACE; goto free_return; } if (dfa->nbackref) { lim_states = re_malloc (re_dfastate_t *, match_last + 1); if (BE (lim_states == NULL, 0)) { ret = REG_ESPACE; goto free_return; } while (1) { memset (lim_states, '\0', sizeof (re_dfastate_t *) * (match_last + 1)); sift_ctx_init (&sctx, sifted_states, lim_states, halt_node, match_last); ret = sift_states_backward (mctx, &sctx); re_node_set_free (&sctx.limits); if (BE (ret != REG_NOERROR, 0)) goto free_return; if (sifted_states[0] != NULL || lim_states[0] != NULL) break; do { --match_last; if (match_last < 0) { ret = REG_NOMATCH; goto free_return; } } while (mctx->state_log[match_last] == NULL || !mctx->state_log[match_last]->halt); halt_node = check_halt_state_context (mctx, mctx->state_log[match_last], match_last); } ret = merge_state_array (dfa, sifted_states, lim_states, match_last + 1); re_free (lim_states); lim_states = NULL; if (BE (ret != REG_NOERROR, 0)) goto free_return; } else { sift_ctx_init (&sctx, sifted_states, lim_states, halt_node, match_last); ret = sift_states_backward (mctx, &sctx); re_node_set_free (&sctx.limits); if (BE (ret != REG_NOERROR, 0)) goto free_return; if (sifted_states[0] == NULL) { ret = REG_NOMATCH; goto free_return; } } re_free (mctx->state_log); mctx->state_log = sifted_states; sifted_states = NULL; mctx->last_node = halt_node; mctx->match_last = match_last; ret = REG_NOERROR; free_return: re_free (sifted_states); re_free (lim_states); return ret; } /* Acquire an initial state and return it. We must select appropriate initial state depending on the context, since initial states may have constraints like "\<", "^", etc.. */ static inline re_dfastate_t * __attribute__ ((always_inline)) internal_function acquire_init_state_context (reg_errcode_t *err, const re_match_context_t *mctx, Idx idx) { const re_dfa_t *const dfa = mctx->dfa; if (dfa->init_state->has_constraint) { unsigned int context; context = re_string_context_at (&mctx->input, idx - 1, mctx->eflags); if (IS_WORD_CONTEXT (context)) return dfa->init_state_word; else if (IS_ORDINARY_CONTEXT (context)) return dfa->init_state; else if (IS_BEGBUF_CONTEXT (context) && IS_NEWLINE_CONTEXT (context)) return dfa->init_state_begbuf; else if (IS_NEWLINE_CONTEXT (context)) return dfa->init_state_nl; else if (IS_BEGBUF_CONTEXT (context)) { /* It is relatively rare case, then calculate on demand. */ return re_acquire_state_context (err, dfa, dfa->init_state->entrance_nodes, context); } else /* Must not happen? */ return dfa->init_state; } else return dfa->init_state; } /* Check whether the regular expression match input string INPUT or not, and return the index where the matching end. Return -1 if there is no match, and return -2 in case of an error. FL_LONGEST_MATCH means we want the POSIX longest matching. If P_MATCH_FIRST is not NULL, and the match fails, it is set to the next place where we may want to try matching. Note that the matcher assumes that the matching starts from the current index of the buffer. */ static Idx internal_function __attribute_warn_unused_result__ check_matching (re_match_context_t *mctx, bool fl_longest_match, Idx *p_match_first) { const re_dfa_t *const dfa = mctx->dfa; reg_errcode_t err; Idx match = 0; Idx match_last = -1; Idx cur_str_idx = re_string_cur_idx (&mctx->input); re_dfastate_t *cur_state; bool at_init_state = p_match_first != NULL; Idx next_start_idx = cur_str_idx; err = REG_NOERROR; cur_state = acquire_init_state_context (&err, mctx, cur_str_idx); /* An initial state must not be NULL (invalid). */ if (BE (cur_state == NULL, 0)) { assert (err == REG_ESPACE); return -2; } if (mctx->state_log != NULL) { mctx->state_log[cur_str_idx] = cur_state; /* Check OP_OPEN_SUBEXP in the initial state in case that we use them later. E.g. Processing back references. */ if (BE (dfa->nbackref, 0)) { at_init_state = false; err = check_subexp_matching_top (mctx, &cur_state->nodes, 0); if (BE (err != REG_NOERROR, 0)) return err; if (cur_state->has_backref) { err = transit_state_bkref (mctx, &cur_state->nodes); if (BE (err != REG_NOERROR, 0)) return err; } } } /* If the RE accepts NULL string. */ if (BE (cur_state->halt, 0)) { if (!cur_state->has_constraint || check_halt_state_context (mctx, cur_state, cur_str_idx)) { if (!fl_longest_match) return cur_str_idx; else { match_last = cur_str_idx; match = 1; } } } while (!re_string_eoi (&mctx->input)) { re_dfastate_t *old_state = cur_state; Idx next_char_idx = re_string_cur_idx (&mctx->input) + 1; if ((BE (next_char_idx >= mctx->input.bufs_len, 0) && mctx->input.bufs_len < mctx->input.len) || (BE (next_char_idx >= mctx->input.valid_len, 0) && mctx->input.valid_len < mctx->input.len)) { err = extend_buffers (mctx, next_char_idx + 1); if (BE (err != REG_NOERROR, 0)) { assert (err == REG_ESPACE); return -2; } } cur_state = transit_state (&err, mctx, cur_state); if (mctx->state_log != NULL) cur_state = merge_state_with_log (&err, mctx, cur_state); if (cur_state == NULL) { /* Reached the invalid state or an error. Try to recover a valid state using the state log, if available and if we have not already found a valid (even if not the longest) match. */ if (BE (err != REG_NOERROR, 0)) return -2; if (mctx->state_log == NULL || (match && !fl_longest_match) || (cur_state = find_recover_state (&err, mctx)) == NULL) break; } if (BE (at_init_state, 0)) { if (old_state == cur_state) next_start_idx = next_char_idx; else at_init_state = false; } if (cur_state->halt) { /* Reached a halt state. Check the halt state can satisfy the current context. */ if (!cur_state->has_constraint || check_halt_state_context (mctx, cur_state, re_string_cur_idx (&mctx->input))) { /* We found an appropriate halt state. */ match_last = re_string_cur_idx (&mctx->input); match = 1; /* We found a match, do not modify match_first below. */ p_match_first = NULL; if (!fl_longest_match) break; } } } if (p_match_first) *p_match_first += next_start_idx; return match_last; } /* Check NODE match the current context. */ static bool internal_function check_halt_node_context (const re_dfa_t *dfa, Idx node, unsigned int context) { re_token_type_t type = dfa->nodes[node].type; unsigned int constraint = dfa->nodes[node].constraint; if (type != END_OF_RE) return false; if (!constraint) return true; if (NOT_SATISFY_NEXT_CONSTRAINT (constraint, context)) return false; return true; } /* Check the halt state STATE match the current context. Return 0 if not match, if the node, STATE has, is a halt node and match the context, return the node. */ static Idx internal_function check_halt_state_context (const re_match_context_t *mctx, const re_dfastate_t *state, Idx idx) { Idx i; unsigned int context; #ifdef DEBUG assert (state->halt); #endif context = re_string_context_at (&mctx->input, idx, mctx->eflags); for (i = 0; i < state->nodes.nelem; ++i) if (check_halt_node_context (mctx->dfa, state->nodes.elems[i], context)) return state->nodes.elems[i]; return 0; } /* Compute the next node to which "NFA" transit from NODE("NFA" is a NFA corresponding to the DFA). Return the destination node, and update EPS_VIA_NODES; return -1 in case of errors. */ static Idx internal_function proceed_next_node (const re_match_context_t *mctx, Idx nregs, regmatch_t *regs, Idx *pidx, Idx node, re_node_set *eps_via_nodes, struct re_fail_stack_t *fs) { const re_dfa_t *const dfa = mctx->dfa; Idx i; bool ok; if (IS_EPSILON_NODE (dfa->nodes[node].type)) { re_node_set *cur_nodes = &mctx->state_log[*pidx]->nodes; re_node_set *edests = &dfa->edests[node]; Idx dest_node; ok = re_node_set_insert (eps_via_nodes, node); if (BE (! ok, 0)) return -2; /* Pick up a valid destination, or return -1 if none is found. */ for (dest_node = -1, i = 0; i < edests->nelem; ++i) { Idx candidate = edests->elems[i]; if (!re_node_set_contains (cur_nodes, candidate)) continue; if (dest_node == -1) dest_node = candidate; else { /* In order to avoid infinite loop like "(a*)*", return the second epsilon-transition if the first was already considered. */ if (re_node_set_contains (eps_via_nodes, dest_node)) return candidate; /* Otherwise, push the second epsilon-transition on the fail stack. */ else if (fs != NULL && push_fail_stack (fs, *pidx, candidate, nregs, regs, eps_via_nodes)) return -2; /* We know we are going to exit. */ break; } } return dest_node; } else { Idx naccepted = 0; re_token_type_t type = dfa->nodes[node].type; #ifdef RE_ENABLE_I18N if (dfa->nodes[node].accept_mb) naccepted = check_node_accept_bytes (dfa, node, &mctx->input, *pidx); else #endif /* RE_ENABLE_I18N */ if (type == OP_BACK_REF) { Idx subexp_idx = dfa->nodes[node].opr.idx + 1; naccepted = regs[subexp_idx].rm_eo - regs[subexp_idx].rm_so; if (fs != NULL) { if (regs[subexp_idx].rm_so == -1 || regs[subexp_idx].rm_eo == -1) return -1; else if (naccepted) { char *buf = (char *) re_string_get_buffer (&mctx->input); if (memcmp (buf + regs[subexp_idx].rm_so, buf + *pidx, naccepted) != 0) return -1; } } if (naccepted == 0) { Idx dest_node; ok = re_node_set_insert (eps_via_nodes, node); if (BE (! ok, 0)) return -2; dest_node = dfa->edests[node].elems[0]; if (re_node_set_contains (&mctx->state_log[*pidx]->nodes, dest_node)) return dest_node; } } if (naccepted != 0 || check_node_accept (mctx, dfa->nodes + node, *pidx)) { Idx dest_node = dfa->nexts[node]; *pidx = (naccepted == 0) ? *pidx + 1 : *pidx + naccepted; if (fs && (*pidx > mctx->match_last || mctx->state_log[*pidx] == NULL || !re_node_set_contains (&mctx->state_log[*pidx]->nodes, dest_node))) return -1; re_node_set_empty (eps_via_nodes); return dest_node; } } return -1; } static reg_errcode_t internal_function __attribute_warn_unused_result__ push_fail_stack (struct re_fail_stack_t *fs, Idx str_idx, Idx dest_node, Idx nregs, regmatch_t *regs, re_node_set *eps_via_nodes) { reg_errcode_t err; Idx num = fs->num++; if (fs->num == fs->alloc) { struct re_fail_stack_ent_t *new_array; new_array = realloc (fs->stack, (sizeof (struct re_fail_stack_ent_t) * fs->alloc * 2)); if (new_array == NULL) return REG_ESPACE; fs->alloc *= 2; fs->stack = new_array; } fs->stack[num].idx = str_idx; fs->stack[num].node = dest_node; fs->stack[num].regs = re_malloc (regmatch_t, nregs); if (fs->stack[num].regs == NULL) return REG_ESPACE; memcpy (fs->stack[num].regs, regs, sizeof (regmatch_t) * nregs); err = re_node_set_init_copy (&fs->stack[num].eps_via_nodes, eps_via_nodes); return err; } static Idx internal_function pop_fail_stack (struct re_fail_stack_t *fs, Idx *pidx, Idx nregs, regmatch_t *regs, re_node_set *eps_via_nodes) { Idx num = --fs->num; assert (num >= 0); *pidx = fs->stack[num].idx; memcpy (regs, fs->stack[num].regs, sizeof (regmatch_t) * nregs); re_node_set_free (eps_via_nodes); re_free (fs->stack[num].regs); *eps_via_nodes = fs->stack[num].eps_via_nodes; return fs->stack[num].node; } /* Set the positions where the subexpressions are starts/ends to registers PMATCH. Note: We assume that pmatch[0] is already set, and pmatch[i].rm_so == pmatch[i].rm_eo == -1 for 0 < i < nmatch. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ set_regs (const regex_t *preg, const re_match_context_t *mctx, size_t nmatch, regmatch_t *pmatch, bool fl_backtrack) { const re_dfa_t *dfa = preg->buffer; Idx idx, cur_node; re_node_set eps_via_nodes; struct re_fail_stack_t *fs; struct re_fail_stack_t fs_body = { 0, 2, NULL }; regmatch_t *prev_idx_match; bool prev_idx_match_malloced = false; #ifdef DEBUG assert (nmatch > 1); assert (mctx->state_log != NULL); #endif if (fl_backtrack) { fs = &fs_body; fs->stack = re_malloc (struct re_fail_stack_ent_t, fs->alloc); if (fs->stack == NULL) return REG_ESPACE; } else fs = NULL; cur_node = dfa->init_node; re_node_set_init_empty (&eps_via_nodes); if (__libc_use_alloca (nmatch * sizeof (regmatch_t))) prev_idx_match = (regmatch_t *) alloca (nmatch * sizeof (regmatch_t)); else { prev_idx_match = re_malloc (regmatch_t, nmatch); if (prev_idx_match == NULL) { free_fail_stack_return (fs); return REG_ESPACE; } prev_idx_match_malloced = true; } memcpy (prev_idx_match, pmatch, sizeof (regmatch_t) * nmatch); for (idx = pmatch[0].rm_so; idx <= pmatch[0].rm_eo ;) { update_regs (dfa, pmatch, prev_idx_match, cur_node, idx, nmatch); if (idx == pmatch[0].rm_eo && cur_node == mctx->last_node) { Idx reg_idx; if (fs) { for (reg_idx = 0; reg_idx < nmatch; ++reg_idx) if (pmatch[reg_idx].rm_so > -1 && pmatch[reg_idx].rm_eo == -1) break; if (reg_idx == nmatch) { re_node_set_free (&eps_via_nodes); if (prev_idx_match_malloced) re_free (prev_idx_match); return free_fail_stack_return (fs); } cur_node = pop_fail_stack (fs, &idx, nmatch, pmatch, &eps_via_nodes); } else { re_node_set_free (&eps_via_nodes); if (prev_idx_match_malloced) re_free (prev_idx_match); return REG_NOERROR; } } /* Proceed to next node. */ cur_node = proceed_next_node (mctx, nmatch, pmatch, &idx, cur_node, &eps_via_nodes, fs); if (BE (cur_node < 0, 0)) { if (BE (cur_node == -2, 0)) { re_node_set_free (&eps_via_nodes); if (prev_idx_match_malloced) re_free (prev_idx_match); free_fail_stack_return (fs); return REG_ESPACE; } if (fs) cur_node = pop_fail_stack (fs, &idx, nmatch, pmatch, &eps_via_nodes); else { re_node_set_free (&eps_via_nodes); if (prev_idx_match_malloced) re_free (prev_idx_match); return REG_NOMATCH; } } } re_node_set_free (&eps_via_nodes); if (prev_idx_match_malloced) re_free (prev_idx_match); return free_fail_stack_return (fs); } static reg_errcode_t internal_function free_fail_stack_return (struct re_fail_stack_t *fs) { if (fs) { Idx fs_idx; for (fs_idx = 0; fs_idx < fs->num; ++fs_idx) { re_node_set_free (&fs->stack[fs_idx].eps_via_nodes); re_free (fs->stack[fs_idx].regs); } re_free (fs->stack); } return REG_NOERROR; } static void internal_function update_regs (const re_dfa_t *dfa, regmatch_t *pmatch, regmatch_t *prev_idx_match, Idx cur_node, Idx cur_idx, Idx nmatch) { int type = dfa->nodes[cur_node].type; if (type == OP_OPEN_SUBEXP) { Idx reg_num = dfa->nodes[cur_node].opr.idx + 1; /* We are at the first node of this sub expression. */ if (reg_num < nmatch) { pmatch[reg_num].rm_so = cur_idx; pmatch[reg_num].rm_eo = -1; } } else if (type == OP_CLOSE_SUBEXP) { Idx reg_num = dfa->nodes[cur_node].opr.idx + 1; if (reg_num < nmatch) { /* We are at the last node of this sub expression. */ if (pmatch[reg_num].rm_so < cur_idx) { pmatch[reg_num].rm_eo = cur_idx; /* This is a non-empty match or we are not inside an optional subexpression. Accept this right away. */ memcpy (prev_idx_match, pmatch, sizeof (regmatch_t) * nmatch); } else { if (dfa->nodes[cur_node].opt_subexp && prev_idx_match[reg_num].rm_so != -1) /* We transited through an empty match for an optional subexpression, like (a?)*, and this is not the subexp's first match. Copy back the old content of the registers so that matches of an inner subexpression are undone as well, like in ((a?))*. */ memcpy (pmatch, prev_idx_match, sizeof (regmatch_t) * nmatch); else /* We completed a subexpression, but it may be part of an optional one, so do not update PREV_IDX_MATCH. */ pmatch[reg_num].rm_eo = cur_idx; } } } } /* This function checks the STATE_LOG from the SCTX->last_str_idx to 0 and sift the nodes in each states according to the following rules. Updated state_log will be wrote to STATE_LOG. Rules: We throw away the Node 'a' in the STATE_LOG[STR_IDX] if... 1. When STR_IDX == MATCH_LAST(the last index in the state_log): If 'a' isn't the LAST_NODE and 'a' can't epsilon transit to the LAST_NODE, we throw away the node 'a'. 2. When 0 <= STR_IDX < MATCH_LAST and 'a' accepts string 's' and transit to 'b': i. If 'b' isn't in the STATE_LOG[STR_IDX+strlen('s')], we throw away the node 'a'. ii. If 'b' is in the STATE_LOG[STR_IDX+strlen('s')] but 'b' is thrown away, we throw away the node 'a'. 3. When 0 <= STR_IDX < MATCH_LAST and 'a' epsilon transit to 'b': i. If 'b' isn't in the STATE_LOG[STR_IDX], we throw away the node 'a'. ii. If 'b' is in the STATE_LOG[STR_IDX] but 'b' is thrown away, we throw away the node 'a'. */ #define STATE_NODE_CONTAINS(state,node) \ ((state) != NULL && re_node_set_contains (&(state)->nodes, node)) static reg_errcode_t internal_function sift_states_backward (const re_match_context_t *mctx, re_sift_context_t *sctx) { reg_errcode_t err; int null_cnt = 0; Idx str_idx = sctx->last_str_idx; re_node_set cur_dest; #ifdef DEBUG assert (mctx->state_log != NULL && mctx->state_log[str_idx] != NULL); #endif /* Build sifted state_log[str_idx]. It has the nodes which can epsilon transit to the last_node and the last_node itself. */ err = re_node_set_init_1 (&cur_dest, sctx->last_node); if (BE (err != REG_NOERROR, 0)) return err; err = update_cur_sifted_state (mctx, sctx, str_idx, &cur_dest); if (BE (err != REG_NOERROR, 0)) goto free_return; /* Then check each states in the state_log. */ while (str_idx > 0) { /* Update counters. */ null_cnt = (sctx->sifted_states[str_idx] == NULL) ? null_cnt + 1 : 0; if (null_cnt > mctx->max_mb_elem_len) { memset (sctx->sifted_states, '\0', sizeof (re_dfastate_t *) * str_idx); re_node_set_free (&cur_dest); return REG_NOERROR; } re_node_set_empty (&cur_dest); --str_idx; if (mctx->state_log[str_idx]) { err = build_sifted_states (mctx, sctx, str_idx, &cur_dest); if (BE (err != REG_NOERROR, 0)) goto free_return; } /* Add all the nodes which satisfy the following conditions: - It can epsilon transit to a node in CUR_DEST. - It is in CUR_SRC. And update state_log. */ err = update_cur_sifted_state (mctx, sctx, str_idx, &cur_dest); if (BE (err != REG_NOERROR, 0)) goto free_return; } err = REG_NOERROR; free_return: re_node_set_free (&cur_dest); return err; } static reg_errcode_t internal_function __attribute_warn_unused_result__ build_sifted_states (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx str_idx, re_node_set *cur_dest) { const re_dfa_t *const dfa = mctx->dfa; const re_node_set *cur_src = &mctx->state_log[str_idx]->non_eps_nodes; Idx i; /* Then build the next sifted state. We build the next sifted state on 'cur_dest', and update 'sifted_states[str_idx]' with 'cur_dest'. Note: 'cur_dest' is the sifted state from 'state_log[str_idx + 1]'. 'cur_src' points the node_set of the old 'state_log[str_idx]' (with the epsilon nodes pre-filtered out). */ for (i = 0; i < cur_src->nelem; i++) { Idx prev_node = cur_src->elems[i]; int naccepted = 0; bool ok; #ifdef DEBUG re_token_type_t type = dfa->nodes[prev_node].type; assert (!IS_EPSILON_NODE (type)); #endif #ifdef RE_ENABLE_I18N /* If the node may accept "multi byte". */ if (dfa->nodes[prev_node].accept_mb) naccepted = sift_states_iter_mb (mctx, sctx, prev_node, str_idx, sctx->last_str_idx); #endif /* RE_ENABLE_I18N */ /* We don't check backreferences here. See update_cur_sifted_state(). */ if (!naccepted && check_node_accept (mctx, dfa->nodes + prev_node, str_idx) && STATE_NODE_CONTAINS (sctx->sifted_states[str_idx + 1], dfa->nexts[prev_node])) naccepted = 1; if (naccepted == 0) continue; if (sctx->limits.nelem) { Idx to_idx = str_idx + naccepted; if (check_dst_limits (mctx, &sctx->limits, dfa->nexts[prev_node], to_idx, prev_node, str_idx)) continue; } ok = re_node_set_insert (cur_dest, prev_node); if (BE (! ok, 0)) return REG_ESPACE; } return REG_NOERROR; } /* Helper functions. */ static reg_errcode_t internal_function clean_state_log_if_needed (re_match_context_t *mctx, Idx next_state_log_idx) { Idx top = mctx->state_log_top; if ((next_state_log_idx >= mctx->input.bufs_len && mctx->input.bufs_len < mctx->input.len) || (next_state_log_idx >= mctx->input.valid_len && mctx->input.valid_len < mctx->input.len)) { reg_errcode_t err; err = extend_buffers (mctx, next_state_log_idx + 1); if (BE (err != REG_NOERROR, 0)) return err; } if (top < next_state_log_idx) { memset (mctx->state_log + top + 1, '\0', sizeof (re_dfastate_t *) * (next_state_log_idx - top)); mctx->state_log_top = next_state_log_idx; } return REG_NOERROR; } static reg_errcode_t internal_function merge_state_array (const re_dfa_t *dfa, re_dfastate_t **dst, re_dfastate_t **src, Idx num) { Idx st_idx; reg_errcode_t err; for (st_idx = 0; st_idx < num; ++st_idx) { if (dst[st_idx] == NULL) dst[st_idx] = src[st_idx]; else if (src[st_idx] != NULL) { re_node_set merged_set; err = re_node_set_init_union (&merged_set, &dst[st_idx]->nodes, &src[st_idx]->nodes); if (BE (err != REG_NOERROR, 0)) return err; dst[st_idx] = re_acquire_state (&err, dfa, &merged_set); re_node_set_free (&merged_set); if (BE (err != REG_NOERROR, 0)) return err; } } return REG_NOERROR; } static reg_errcode_t internal_function update_cur_sifted_state (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx str_idx, re_node_set *dest_nodes) { const re_dfa_t *const dfa = mctx->dfa; reg_errcode_t err = REG_NOERROR; const re_node_set *candidates; candidates = ((mctx->state_log[str_idx] == NULL) ? NULL : &mctx->state_log[str_idx]->nodes); if (dest_nodes->nelem == 0) sctx->sifted_states[str_idx] = NULL; else { if (candidates) { /* At first, add the nodes which can epsilon transit to a node in DEST_NODE. */ err = add_epsilon_src_nodes (dfa, dest_nodes, candidates); if (BE (err != REG_NOERROR, 0)) return err; /* Then, check the limitations in the current sift_context. */ if (sctx->limits.nelem) { err = check_subexp_limits (dfa, dest_nodes, candidates, &sctx->limits, mctx->bkref_ents, str_idx); if (BE (err != REG_NOERROR, 0)) return err; } } sctx->sifted_states[str_idx] = re_acquire_state (&err, dfa, dest_nodes); if (BE (err != REG_NOERROR, 0)) return err; } if (candidates && mctx->state_log[str_idx]->has_backref) { err = sift_states_bkref (mctx, sctx, str_idx, candidates); if (BE (err != REG_NOERROR, 0)) return err; } return REG_NOERROR; } static reg_errcode_t internal_function __attribute_warn_unused_result__ add_epsilon_src_nodes (const re_dfa_t *dfa, re_node_set *dest_nodes, const re_node_set *candidates) { reg_errcode_t err = REG_NOERROR; Idx i; re_dfastate_t *state = re_acquire_state (&err, dfa, dest_nodes); if (BE (err != REG_NOERROR, 0)) return err; if (!state->inveclosure.alloc) { err = re_node_set_alloc (&state->inveclosure, dest_nodes->nelem); if (BE (err != REG_NOERROR, 0)) return REG_ESPACE; for (i = 0; i < dest_nodes->nelem; i++) { err = re_node_set_merge (&state->inveclosure, dfa->inveclosures + dest_nodes->elems[i]); if (BE (err != REG_NOERROR, 0)) return REG_ESPACE; } } return re_node_set_add_intersect (dest_nodes, candidates, &state->inveclosure); } static reg_errcode_t internal_function sub_epsilon_src_nodes (const re_dfa_t *dfa, Idx node, re_node_set *dest_nodes, const re_node_set *candidates) { Idx ecl_idx; reg_errcode_t err; re_node_set *inv_eclosure = dfa->inveclosures + node; re_node_set except_nodes; re_node_set_init_empty (&except_nodes); for (ecl_idx = 0; ecl_idx < inv_eclosure->nelem; ++ecl_idx) { Idx cur_node = inv_eclosure->elems[ecl_idx]; if (cur_node == node) continue; if (IS_EPSILON_NODE (dfa->nodes[cur_node].type)) { Idx edst1 = dfa->edests[cur_node].elems[0]; Idx edst2 = ((dfa->edests[cur_node].nelem > 1) ? dfa->edests[cur_node].elems[1] : -1); if ((!re_node_set_contains (inv_eclosure, edst1) && re_node_set_contains (dest_nodes, edst1)) || (edst2 > 0 && !re_node_set_contains (inv_eclosure, edst2) && re_node_set_contains (dest_nodes, edst2))) { err = re_node_set_add_intersect (&except_nodes, candidates, dfa->inveclosures + cur_node); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&except_nodes); return err; } } } } for (ecl_idx = 0; ecl_idx < inv_eclosure->nelem; ++ecl_idx) { Idx cur_node = inv_eclosure->elems[ecl_idx]; if (!re_node_set_contains (&except_nodes, cur_node)) { Idx idx = re_node_set_contains (dest_nodes, cur_node) - 1; re_node_set_remove_at (dest_nodes, idx); } } re_node_set_free (&except_nodes); return REG_NOERROR; } static bool internal_function check_dst_limits (const re_match_context_t *mctx, const re_node_set *limits, Idx dst_node, Idx dst_idx, Idx src_node, Idx src_idx) { const re_dfa_t *const dfa = mctx->dfa; Idx lim_idx, src_pos, dst_pos; Idx dst_bkref_idx = search_cur_bkref_entry (mctx, dst_idx); Idx src_bkref_idx = search_cur_bkref_entry (mctx, src_idx); for (lim_idx = 0; lim_idx < limits->nelem; ++lim_idx) { Idx subexp_idx; struct re_backref_cache_entry *ent; ent = mctx->bkref_ents + limits->elems[lim_idx]; subexp_idx = dfa->nodes[ent->node].opr.idx; dst_pos = check_dst_limits_calc_pos (mctx, limits->elems[lim_idx], subexp_idx, dst_node, dst_idx, dst_bkref_idx); src_pos = check_dst_limits_calc_pos (mctx, limits->elems[lim_idx], subexp_idx, src_node, src_idx, src_bkref_idx); /* In case of: ( ) ( ) ( ) */ if (src_pos == dst_pos) continue; /* This is unrelated limitation. */ else return true; } return false; } static int internal_function check_dst_limits_calc_pos_1 (const re_match_context_t *mctx, int boundaries, Idx subexp_idx, Idx from_node, Idx bkref_idx) { const re_dfa_t *const dfa = mctx->dfa; const re_node_set *eclosures = dfa->eclosures + from_node; Idx node_idx; /* Else, we are on the boundary: examine the nodes on the epsilon closure. */ for (node_idx = 0; node_idx < eclosures->nelem; ++node_idx) { Idx node = eclosures->elems[node_idx]; switch (dfa->nodes[node].type) { case OP_BACK_REF: if (bkref_idx != -1) { struct re_backref_cache_entry *ent = mctx->bkref_ents + bkref_idx; do { Idx dst; int cpos; if (ent->node != node) continue; if (subexp_idx < BITSET_WORD_BITS && !(ent->eps_reachable_subexps_map & ((bitset_word_t) 1 << subexp_idx))) continue; /* Recurse trying to reach the OP_OPEN_SUBEXP and OP_CLOSE_SUBEXP cases below. But, if the destination node is the same node as the source node, don't recurse because it would cause an infinite loop: a regex that exhibits this behavior is ()\1*\1* */ dst = dfa->edests[node].elems[0]; if (dst == from_node) { if (boundaries & 1) return -1; else /* if (boundaries & 2) */ return 0; } cpos = check_dst_limits_calc_pos_1 (mctx, boundaries, subexp_idx, dst, bkref_idx); if (cpos == -1 /* && (boundaries & 1) */) return -1; if (cpos == 0 && (boundaries & 2)) return 0; if (subexp_idx < BITSET_WORD_BITS) ent->eps_reachable_subexps_map &= ~((bitset_word_t) 1 << subexp_idx); } while (ent++->more); } break; case OP_OPEN_SUBEXP: if ((boundaries & 1) && subexp_idx == dfa->nodes[node].opr.idx) return -1; break; case OP_CLOSE_SUBEXP: if ((boundaries & 2) && subexp_idx == dfa->nodes[node].opr.idx) return 0; break; default: break; } } return (boundaries & 2) ? 1 : 0; } static int internal_function check_dst_limits_calc_pos (const re_match_context_t *mctx, Idx limit, Idx subexp_idx, Idx from_node, Idx str_idx, Idx bkref_idx) { struct re_backref_cache_entry *lim = mctx->bkref_ents + limit; int boundaries; /* If we are outside the range of the subexpression, return -1 or 1. */ if (str_idx < lim->subexp_from) return -1; if (lim->subexp_to < str_idx) return 1; /* If we are within the subexpression, return 0. */ boundaries = (str_idx == lim->subexp_from); boundaries |= (str_idx == lim->subexp_to) << 1; if (boundaries == 0) return 0; /* Else, examine epsilon closure. */ return check_dst_limits_calc_pos_1 (mctx, boundaries, subexp_idx, from_node, bkref_idx); } /* Check the limitations of sub expressions LIMITS, and remove the nodes which are against limitations from DEST_NODES. */ static reg_errcode_t internal_function check_subexp_limits (const re_dfa_t *dfa, re_node_set *dest_nodes, const re_node_set *candidates, re_node_set *limits, struct re_backref_cache_entry *bkref_ents, Idx str_idx) { reg_errcode_t err; Idx node_idx, lim_idx; for (lim_idx = 0; lim_idx < limits->nelem; ++lim_idx) { Idx subexp_idx; struct re_backref_cache_entry *ent; ent = bkref_ents + limits->elems[lim_idx]; if (str_idx <= ent->subexp_from || ent->str_idx < str_idx) continue; /* This is unrelated limitation. */ subexp_idx = dfa->nodes[ent->node].opr.idx; if (ent->subexp_to == str_idx) { Idx ops_node = -1; Idx cls_node = -1; for (node_idx = 0; node_idx < dest_nodes->nelem; ++node_idx) { Idx node = dest_nodes->elems[node_idx]; re_token_type_t type = dfa->nodes[node].type; if (type == OP_OPEN_SUBEXP && subexp_idx == dfa->nodes[node].opr.idx) ops_node = node; else if (type == OP_CLOSE_SUBEXP && subexp_idx == dfa->nodes[node].opr.idx) cls_node = node; } /* Check the limitation of the open subexpression. */ /* Note that (ent->subexp_to = str_idx != ent->subexp_from). */ if (ops_node >= 0) { err = sub_epsilon_src_nodes (dfa, ops_node, dest_nodes, candidates); if (BE (err != REG_NOERROR, 0)) return err; } /* Check the limitation of the close subexpression. */ if (cls_node >= 0) for (node_idx = 0; node_idx < dest_nodes->nelem; ++node_idx) { Idx node = dest_nodes->elems[node_idx]; if (!re_node_set_contains (dfa->inveclosures + node, cls_node) && !re_node_set_contains (dfa->eclosures + node, cls_node)) { /* It is against this limitation. Remove it form the current sifted state. */ err = sub_epsilon_src_nodes (dfa, node, dest_nodes, candidates); if (BE (err != REG_NOERROR, 0)) return err; --node_idx; } } } else /* (ent->subexp_to != str_idx) */ { for (node_idx = 0; node_idx < dest_nodes->nelem; ++node_idx) { Idx node = dest_nodes->elems[node_idx]; re_token_type_t type = dfa->nodes[node].type; if (type == OP_CLOSE_SUBEXP || type == OP_OPEN_SUBEXP) { if (subexp_idx != dfa->nodes[node].opr.idx) continue; /* It is against this limitation. Remove it form the current sifted state. */ err = sub_epsilon_src_nodes (dfa, node, dest_nodes, candidates); if (BE (err != REG_NOERROR, 0)) return err; } } } } return REG_NOERROR; } static reg_errcode_t internal_function __attribute_warn_unused_result__ sift_states_bkref (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx str_idx, const re_node_set *candidates) { const re_dfa_t *const dfa = mctx->dfa; reg_errcode_t err; Idx node_idx, node; re_sift_context_t local_sctx; Idx first_idx = search_cur_bkref_entry (mctx, str_idx); if (first_idx == -1) return REG_NOERROR; local_sctx.sifted_states = NULL; /* Mark that it hasn't been initialized. */ for (node_idx = 0; node_idx < candidates->nelem; ++node_idx) { Idx enabled_idx; re_token_type_t type; struct re_backref_cache_entry *entry; node = candidates->elems[node_idx]; type = dfa->nodes[node].type; /* Avoid infinite loop for the REs like "()\1+". */ if (node == sctx->last_node && str_idx == sctx->last_str_idx) continue; if (type != OP_BACK_REF) continue; entry = mctx->bkref_ents + first_idx; enabled_idx = first_idx; do { Idx subexp_len; Idx to_idx; Idx dst_node; bool ok; re_dfastate_t *cur_state; if (entry->node != node) continue; subexp_len = entry->subexp_to - entry->subexp_from; to_idx = str_idx + subexp_len; dst_node = (subexp_len ? dfa->nexts[node] : dfa->edests[node].elems[0]); if (to_idx > sctx->last_str_idx || sctx->sifted_states[to_idx] == NULL || !STATE_NODE_CONTAINS (sctx->sifted_states[to_idx], dst_node) || check_dst_limits (mctx, &sctx->limits, node, str_idx, dst_node, to_idx)) continue; if (local_sctx.sifted_states == NULL) { local_sctx = *sctx; err = re_node_set_init_copy (&local_sctx.limits, &sctx->limits); if (BE (err != REG_NOERROR, 0)) goto free_return; } local_sctx.last_node = node; local_sctx.last_str_idx = str_idx; ok = re_node_set_insert (&local_sctx.limits, enabled_idx); if (BE (! ok, 0)) { err = REG_ESPACE; goto free_return; } cur_state = local_sctx.sifted_states[str_idx]; err = sift_states_backward (mctx, &local_sctx); if (BE (err != REG_NOERROR, 0)) goto free_return; if (sctx->limited_states != NULL) { err = merge_state_array (dfa, sctx->limited_states, local_sctx.sifted_states, str_idx + 1); if (BE (err != REG_NOERROR, 0)) goto free_return; } local_sctx.sifted_states[str_idx] = cur_state; re_node_set_remove (&local_sctx.limits, enabled_idx); /* mctx->bkref_ents may have changed, reload the pointer. */ entry = mctx->bkref_ents + enabled_idx; } while (enabled_idx++, entry++->more); } err = REG_NOERROR; free_return: if (local_sctx.sifted_states != NULL) { re_node_set_free (&local_sctx.limits); } return err; } #ifdef RE_ENABLE_I18N static int internal_function sift_states_iter_mb (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx node_idx, Idx str_idx, Idx max_str_idx) { const re_dfa_t *const dfa = mctx->dfa; int naccepted; /* Check the node can accept "multi byte". */ naccepted = check_node_accept_bytes (dfa, node_idx, &mctx->input, str_idx); if (naccepted > 0 && str_idx + naccepted <= max_str_idx && !STATE_NODE_CONTAINS (sctx->sifted_states[str_idx + naccepted], dfa->nexts[node_idx])) /* The node can't accept the "multi byte", or the destination was already thrown away, then the node could't accept the current input "multi byte". */ naccepted = 0; /* Otherwise, it is sure that the node could accept 'naccepted' bytes input. */ return naccepted; } #endif /* RE_ENABLE_I18N */ /* Functions for state transition. */ /* Return the next state to which the current state STATE will transit by accepting the current input byte, and update STATE_LOG if necessary. If STATE can accept a multibyte char/collating element/back reference update the destination of STATE_LOG. */ static re_dfastate_t * internal_function __attribute_warn_unused_result__ transit_state (reg_errcode_t *err, re_match_context_t *mctx, re_dfastate_t *state) { re_dfastate_t **trtable; unsigned char ch; #ifdef RE_ENABLE_I18N /* If the current state can accept multibyte. */ if (BE (state->accept_mb, 0)) { *err = transit_state_mb (mctx, state); if (BE (*err != REG_NOERROR, 0)) return NULL; } #endif /* RE_ENABLE_I18N */ /* Then decide the next state with the single byte. */ #if 0 if (0) /* don't use transition table */ return transit_state_sb (err, mctx, state); #endif /* Use transition table */ ch = re_string_fetch_byte (&mctx->input); for (;;) { trtable = state->trtable; if (BE (trtable != NULL, 1)) return trtable[ch]; trtable = state->word_trtable; if (BE (trtable != NULL, 1)) { unsigned int context; context = re_string_context_at (&mctx->input, re_string_cur_idx (&mctx->input) - 1, mctx->eflags); if (IS_WORD_CONTEXT (context)) return trtable[ch + SBC_MAX]; else return trtable[ch]; } if (!build_trtable (mctx->dfa, state)) { *err = REG_ESPACE; return NULL; } /* Retry, we now have a transition table. */ } } /* Update the state_log if we need */ static re_dfastate_t * internal_function merge_state_with_log (reg_errcode_t *err, re_match_context_t *mctx, re_dfastate_t *next_state) { const re_dfa_t *const dfa = mctx->dfa; Idx cur_idx = re_string_cur_idx (&mctx->input); if (cur_idx > mctx->state_log_top) { mctx->state_log[cur_idx] = next_state; mctx->state_log_top = cur_idx; } else if (mctx->state_log[cur_idx] == 0) { mctx->state_log[cur_idx] = next_state; } else { re_dfastate_t *pstate; unsigned int context; re_node_set next_nodes, *log_nodes, *table_nodes = NULL; /* If (state_log[cur_idx] != 0), it implies that cur_idx is the destination of a multibyte char/collating element/ back reference. Then the next state is the union set of these destinations and the results of the transition table. */ pstate = mctx->state_log[cur_idx]; log_nodes = pstate->entrance_nodes; if (next_state != NULL) { table_nodes = next_state->entrance_nodes; *err = re_node_set_init_union (&next_nodes, table_nodes, log_nodes); if (BE (*err != REG_NOERROR, 0)) return NULL; } else next_nodes = *log_nodes; /* Note: We already add the nodes of the initial state, then we don't need to add them here. */ context = re_string_context_at (&mctx->input, re_string_cur_idx (&mctx->input) - 1, mctx->eflags); next_state = mctx->state_log[cur_idx] = re_acquire_state_context (err, dfa, &next_nodes, context); /* We don't need to check errors here, since the return value of this function is next_state and ERR is already set. */ if (table_nodes != NULL) re_node_set_free (&next_nodes); } if (BE (dfa->nbackref, 0) && next_state != NULL) { /* Check OP_OPEN_SUBEXP in the current state in case that we use them later. We must check them here, since the back references in the next state might use them. */ *err = check_subexp_matching_top (mctx, &next_state->nodes, cur_idx); if (BE (*err != REG_NOERROR, 0)) return NULL; /* If the next state has back references. */ if (next_state->has_backref) { *err = transit_state_bkref (mctx, &next_state->nodes); if (BE (*err != REG_NOERROR, 0)) return NULL; next_state = mctx->state_log[cur_idx]; } } return next_state; } /* Skip bytes in the input that correspond to part of a multi-byte match, then look in the log for a state from which to restart matching. */ static re_dfastate_t * internal_function find_recover_state (reg_errcode_t *err, re_match_context_t *mctx) { re_dfastate_t *cur_state; do { Idx max = mctx->state_log_top; Idx cur_str_idx = re_string_cur_idx (&mctx->input); do { if (++cur_str_idx > max) return NULL; re_string_skip_bytes (&mctx->input, 1); } while (mctx->state_log[cur_str_idx] == NULL); cur_state = merge_state_with_log (err, mctx, NULL); } while (*err == REG_NOERROR && cur_state == NULL); return cur_state; } /* Helper functions for transit_state. */ /* From the node set CUR_NODES, pick up the nodes whose types are OP_OPEN_SUBEXP and which have corresponding back references in the regular expression. And register them to use them later for evaluating the corresponding back references. */ static reg_errcode_t internal_function check_subexp_matching_top (re_match_context_t *mctx, re_node_set *cur_nodes, Idx str_idx) { const re_dfa_t *const dfa = mctx->dfa; Idx node_idx; reg_errcode_t err; /* TODO: This isn't efficient. Because there might be more than one nodes whose types are OP_OPEN_SUBEXP and whose index is SUBEXP_IDX, we must check all nodes. E.g. RE: (a){2} */ for (node_idx = 0; node_idx < cur_nodes->nelem; ++node_idx) { Idx node = cur_nodes->elems[node_idx]; if (dfa->nodes[node].type == OP_OPEN_SUBEXP && dfa->nodes[node].opr.idx < BITSET_WORD_BITS && (dfa->used_bkref_map & ((bitset_word_t) 1 << dfa->nodes[node].opr.idx))) { err = match_ctx_add_subtop (mctx, node, str_idx); if (BE (err != REG_NOERROR, 0)) return err; } } return REG_NOERROR; } #if 0 /* Return the next state to which the current state STATE will transit by accepting the current input byte. */ static re_dfastate_t * transit_state_sb (reg_errcode_t *err, re_match_context_t *mctx, re_dfastate_t *state) { const re_dfa_t *const dfa = mctx->dfa; re_node_set next_nodes; re_dfastate_t *next_state; Idx node_cnt, cur_str_idx = re_string_cur_idx (&mctx->input); unsigned int context; *err = re_node_set_alloc (&next_nodes, state->nodes.nelem + 1); if (BE (*err != REG_NOERROR, 0)) return NULL; for (node_cnt = 0; node_cnt < state->nodes.nelem; ++node_cnt) { Idx cur_node = state->nodes.elems[node_cnt]; if (check_node_accept (mctx, dfa->nodes + cur_node, cur_str_idx)) { *err = re_node_set_merge (&next_nodes, dfa->eclosures + dfa->nexts[cur_node]); if (BE (*err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return NULL; } } } context = re_string_context_at (&mctx->input, cur_str_idx, mctx->eflags); next_state = re_acquire_state_context (err, dfa, &next_nodes, context); /* We don't need to check errors here, since the return value of this function is next_state and ERR is already set. */ re_node_set_free (&next_nodes); re_string_skip_bytes (&mctx->input, 1); return next_state; } #endif #ifdef RE_ENABLE_I18N static reg_errcode_t internal_function transit_state_mb (re_match_context_t *mctx, re_dfastate_t *pstate) { const re_dfa_t *const dfa = mctx->dfa; reg_errcode_t err; Idx i; for (i = 0; i < pstate->nodes.nelem; ++i) { re_node_set dest_nodes, *new_nodes; Idx cur_node_idx = pstate->nodes.elems[i]; int naccepted; Idx dest_idx; unsigned int context; re_dfastate_t *dest_state; if (!dfa->nodes[cur_node_idx].accept_mb) continue; if (dfa->nodes[cur_node_idx].constraint) { context = re_string_context_at (&mctx->input, re_string_cur_idx (&mctx->input), mctx->eflags); if (NOT_SATISFY_NEXT_CONSTRAINT (dfa->nodes[cur_node_idx].constraint, context)) continue; } /* How many bytes the node can accept? */ naccepted = check_node_accept_bytes (dfa, cur_node_idx, &mctx->input, re_string_cur_idx (&mctx->input)); if (naccepted == 0) continue; /* The node can accepts 'naccepted' bytes. */ dest_idx = re_string_cur_idx (&mctx->input) + naccepted; mctx->max_mb_elem_len = ((mctx->max_mb_elem_len < naccepted) ? naccepted : mctx->max_mb_elem_len); err = clean_state_log_if_needed (mctx, dest_idx); if (BE (err != REG_NOERROR, 0)) return err; #ifdef DEBUG assert (dfa->nexts[cur_node_idx] != -1); #endif new_nodes = dfa->eclosures + dfa->nexts[cur_node_idx]; dest_state = mctx->state_log[dest_idx]; if (dest_state == NULL) dest_nodes = *new_nodes; else { err = re_node_set_init_union (&dest_nodes, dest_state->entrance_nodes, new_nodes); if (BE (err != REG_NOERROR, 0)) return err; } context = re_string_context_at (&mctx->input, dest_idx - 1, mctx->eflags); mctx->state_log[dest_idx] = re_acquire_state_context (&err, dfa, &dest_nodes, context); if (dest_state != NULL) re_node_set_free (&dest_nodes); if (BE (mctx->state_log[dest_idx] == NULL && err != REG_NOERROR, 0)) return err; } return REG_NOERROR; } #endif /* RE_ENABLE_I18N */ static reg_errcode_t internal_function transit_state_bkref (re_match_context_t *mctx, const re_node_set *nodes) { const re_dfa_t *const dfa = mctx->dfa; reg_errcode_t err; Idx i; Idx cur_str_idx = re_string_cur_idx (&mctx->input); for (i = 0; i < nodes->nelem; ++i) { Idx dest_str_idx, prev_nelem, bkc_idx; Idx node_idx = nodes->elems[i]; unsigned int context; const re_token_t *node = dfa->nodes + node_idx; re_node_set *new_dest_nodes; /* Check whether 'node' is a backreference or not. */ if (node->type != OP_BACK_REF) continue; if (node->constraint) { context = re_string_context_at (&mctx->input, cur_str_idx, mctx->eflags); if (NOT_SATISFY_NEXT_CONSTRAINT (node->constraint, context)) continue; } /* 'node' is a backreference. Check the substring which the substring matched. */ bkc_idx = mctx->nbkref_ents; err = get_subexp (mctx, node_idx, cur_str_idx); if (BE (err != REG_NOERROR, 0)) goto free_return; /* And add the epsilon closures (which is 'new_dest_nodes') of the backreference to appropriate state_log. */ #ifdef DEBUG assert (dfa->nexts[node_idx] != -1); #endif for (; bkc_idx < mctx->nbkref_ents; ++bkc_idx) { Idx subexp_len; re_dfastate_t *dest_state; struct re_backref_cache_entry *bkref_ent; bkref_ent = mctx->bkref_ents + bkc_idx; if (bkref_ent->node != node_idx || bkref_ent->str_idx != cur_str_idx) continue; subexp_len = bkref_ent->subexp_to - bkref_ent->subexp_from; new_dest_nodes = (subexp_len == 0 ? dfa->eclosures + dfa->edests[node_idx].elems[0] : dfa->eclosures + dfa->nexts[node_idx]); dest_str_idx = (cur_str_idx + bkref_ent->subexp_to - bkref_ent->subexp_from); context = re_string_context_at (&mctx->input, dest_str_idx - 1, mctx->eflags); dest_state = mctx->state_log[dest_str_idx]; prev_nelem = ((mctx->state_log[cur_str_idx] == NULL) ? 0 : mctx->state_log[cur_str_idx]->nodes.nelem); /* Add 'new_dest_node' to state_log. */ if (dest_state == NULL) { mctx->state_log[dest_str_idx] = re_acquire_state_context (&err, dfa, new_dest_nodes, context); if (BE (mctx->state_log[dest_str_idx] == NULL && err != REG_NOERROR, 0)) goto free_return; } else { re_node_set dest_nodes; err = re_node_set_init_union (&dest_nodes, dest_state->entrance_nodes, new_dest_nodes); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&dest_nodes); goto free_return; } mctx->state_log[dest_str_idx] = re_acquire_state_context (&err, dfa, &dest_nodes, context); re_node_set_free (&dest_nodes); if (BE (mctx->state_log[dest_str_idx] == NULL && err != REG_NOERROR, 0)) goto free_return; } /* We need to check recursively if the backreference can epsilon transit. */ if (subexp_len == 0 && mctx->state_log[cur_str_idx]->nodes.nelem > prev_nelem) { err = check_subexp_matching_top (mctx, new_dest_nodes, cur_str_idx); if (BE (err != REG_NOERROR, 0)) goto free_return; err = transit_state_bkref (mctx, new_dest_nodes); if (BE (err != REG_NOERROR, 0)) goto free_return; } } } err = REG_NOERROR; free_return: return err; } /* Enumerate all the candidates which the backreference BKREF_NODE can match at BKREF_STR_IDX, and register them by match_ctx_add_entry(). Note that we might collect inappropriate candidates here. However, the cost of checking them strictly here is too high, then we delay these checking for prune_impossible_nodes(). */ static reg_errcode_t internal_function __attribute_warn_unused_result__ get_subexp (re_match_context_t *mctx, Idx bkref_node, Idx bkref_str_idx) { const re_dfa_t *const dfa = mctx->dfa; Idx subexp_num, sub_top_idx; const char *buf = (const char *) re_string_get_buffer (&mctx->input); /* Return if we have already checked BKREF_NODE at BKREF_STR_IDX. */ Idx cache_idx = search_cur_bkref_entry (mctx, bkref_str_idx); if (cache_idx != -1) { const struct re_backref_cache_entry *entry = mctx->bkref_ents + cache_idx; do if (entry->node == bkref_node) return REG_NOERROR; /* We already checked it. */ while (entry++->more); } subexp_num = dfa->nodes[bkref_node].opr.idx; /* For each sub expression */ for (sub_top_idx = 0; sub_top_idx < mctx->nsub_tops; ++sub_top_idx) { reg_errcode_t err; re_sub_match_top_t *sub_top = mctx->sub_tops[sub_top_idx]; re_sub_match_last_t *sub_last; Idx sub_last_idx, sl_str, bkref_str_off; if (dfa->nodes[sub_top->node].opr.idx != subexp_num) continue; /* It isn't related. */ sl_str = sub_top->str_idx; bkref_str_off = bkref_str_idx; /* At first, check the last node of sub expressions we already evaluated. */ for (sub_last_idx = 0; sub_last_idx < sub_top->nlasts; ++sub_last_idx) { regoff_t sl_str_diff; sub_last = sub_top->lasts[sub_last_idx]; sl_str_diff = sub_last->str_idx - sl_str; /* The matched string by the sub expression match with the substring at the back reference? */ if (sl_str_diff > 0) { if (BE (bkref_str_off + sl_str_diff > mctx->input.valid_len, 0)) { /* Not enough chars for a successful match. */ if (bkref_str_off + sl_str_diff > mctx->input.len) break; err = clean_state_log_if_needed (mctx, bkref_str_off + sl_str_diff); if (BE (err != REG_NOERROR, 0)) return err; buf = (const char *) re_string_get_buffer (&mctx->input); } if (memcmp (buf + bkref_str_off, buf + sl_str, sl_str_diff) != 0) /* We don't need to search this sub expression any more. */ break; } bkref_str_off += sl_str_diff; sl_str += sl_str_diff; err = get_subexp_sub (mctx, sub_top, sub_last, bkref_node, bkref_str_idx); /* Reload buf, since the preceding call might have reallocated the buffer. */ buf = (const char *) re_string_get_buffer (&mctx->input); if (err == REG_NOMATCH) continue; if (BE (err != REG_NOERROR, 0)) return err; } if (sub_last_idx < sub_top->nlasts) continue; if (sub_last_idx > 0) ++sl_str; /* Then, search for the other last nodes of the sub expression. */ for (; sl_str <= bkref_str_idx; ++sl_str) { Idx cls_node; regoff_t sl_str_off; const re_node_set *nodes; sl_str_off = sl_str - sub_top->str_idx; /* The matched string by the sub expression match with the substring at the back reference? */ if (sl_str_off > 0) { if (BE (bkref_str_off >= mctx->input.valid_len, 0)) { /* If we are at the end of the input, we cannot match. */ if (bkref_str_off >= mctx->input.len) break; err = extend_buffers (mctx, bkref_str_off + 1); if (BE (err != REG_NOERROR, 0)) return err; buf = (const char *) re_string_get_buffer (&mctx->input); } if (buf [bkref_str_off++] != buf[sl_str - 1]) break; /* We don't need to search this sub expression any more. */ } if (mctx->state_log[sl_str] == NULL) continue; /* Does this state have a ')' of the sub expression? */ nodes = &mctx->state_log[sl_str]->nodes; cls_node = find_subexp_node (dfa, nodes, subexp_num, OP_CLOSE_SUBEXP); if (cls_node == -1) continue; /* No. */ if (sub_top->path == NULL) { sub_top->path = calloc (sizeof (state_array_t), sl_str - sub_top->str_idx + 1); if (sub_top->path == NULL) return REG_ESPACE; } /* Can the OP_OPEN_SUBEXP node arrive the OP_CLOSE_SUBEXP node in the current context? */ err = check_arrival (mctx, sub_top->path, sub_top->node, sub_top->str_idx, cls_node, sl_str, OP_CLOSE_SUBEXP); if (err == REG_NOMATCH) continue; if (BE (err != REG_NOERROR, 0)) return err; sub_last = match_ctx_add_sublast (sub_top, cls_node, sl_str); if (BE (sub_last == NULL, 0)) return REG_ESPACE; err = get_subexp_sub (mctx, sub_top, sub_last, bkref_node, bkref_str_idx); if (err == REG_NOMATCH) continue; } } return REG_NOERROR; } /* Helper functions for get_subexp(). */ /* Check SUB_LAST can arrive to the back reference BKREF_NODE at BKREF_STR. If it can arrive, register the sub expression expressed with SUB_TOP and SUB_LAST. */ static reg_errcode_t internal_function get_subexp_sub (re_match_context_t *mctx, const re_sub_match_top_t *sub_top, re_sub_match_last_t *sub_last, Idx bkref_node, Idx bkref_str) { reg_errcode_t err; Idx to_idx; /* Can the subexpression arrive the back reference? */ err = check_arrival (mctx, &sub_last->path, sub_last->node, sub_last->str_idx, bkref_node, bkref_str, OP_OPEN_SUBEXP); if (err != REG_NOERROR) return err; err = match_ctx_add_entry (mctx, bkref_node, bkref_str, sub_top->str_idx, sub_last->str_idx); if (BE (err != REG_NOERROR, 0)) return err; to_idx = bkref_str + sub_last->str_idx - sub_top->str_idx; return clean_state_log_if_needed (mctx, to_idx); } /* Find the first node which is '(' or ')' and whose index is SUBEXP_IDX. Search '(' if FL_OPEN, or search ')' otherwise. TODO: This function isn't efficient... Because there might be more than one nodes whose types are OP_OPEN_SUBEXP and whose index is SUBEXP_IDX, we must check all nodes. E.g. RE: (a){2} */ static Idx internal_function find_subexp_node (const re_dfa_t *dfa, const re_node_set *nodes, Idx subexp_idx, int type) { Idx cls_idx; for (cls_idx = 0; cls_idx < nodes->nelem; ++cls_idx) { Idx cls_node = nodes->elems[cls_idx]; const re_token_t *node = dfa->nodes + cls_node; if (node->type == type && node->opr.idx == subexp_idx) return cls_node; } return -1; } /* Check whether the node TOP_NODE at TOP_STR can arrive to the node LAST_NODE at LAST_STR. We record the path onto PATH since it will be heavily reused. Return REG_NOERROR if it can arrive, or REG_NOMATCH otherwise. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ check_arrival (re_match_context_t *mctx, state_array_t *path, Idx top_node, Idx top_str, Idx last_node, Idx last_str, int type) { const re_dfa_t *const dfa = mctx->dfa; reg_errcode_t err = REG_NOERROR; Idx subexp_num, backup_cur_idx, str_idx, null_cnt; re_dfastate_t *cur_state = NULL; re_node_set *cur_nodes, next_nodes; re_dfastate_t **backup_state_log; unsigned int context; subexp_num = dfa->nodes[top_node].opr.idx; /* Extend the buffer if we need. */ if (BE (path->alloc < last_str + mctx->max_mb_elem_len + 1, 0)) { re_dfastate_t **new_array; Idx old_alloc = path->alloc; Idx incr_alloc = last_str + mctx->max_mb_elem_len + 1; Idx new_alloc; if (BE (IDX_MAX - old_alloc < incr_alloc, 0)) return REG_ESPACE; new_alloc = old_alloc + incr_alloc; if (BE (SIZE_MAX / sizeof (re_dfastate_t *) < new_alloc, 0)) return REG_ESPACE; new_array = re_realloc (path->array, re_dfastate_t *, new_alloc); if (BE (new_array == NULL, 0)) return REG_ESPACE; path->array = new_array; path->alloc = new_alloc; memset (new_array + old_alloc, '\0', sizeof (re_dfastate_t *) * (path->alloc - old_alloc)); } str_idx = path->next_idx ? path->next_idx : top_str; /* Temporary modify MCTX. */ backup_state_log = mctx->state_log; backup_cur_idx = mctx->input.cur_idx; mctx->state_log = path->array; mctx->input.cur_idx = str_idx; /* Setup initial node set. */ context = re_string_context_at (&mctx->input, str_idx - 1, mctx->eflags); if (str_idx == top_str) { err = re_node_set_init_1 (&next_nodes, top_node); if (BE (err != REG_NOERROR, 0)) return err; err = check_arrival_expand_ecl (dfa, &next_nodes, subexp_num, type); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } } else { cur_state = mctx->state_log[str_idx]; if (cur_state && cur_state->has_backref) { err = re_node_set_init_copy (&next_nodes, &cur_state->nodes); if (BE (err != REG_NOERROR, 0)) return err; } else re_node_set_init_empty (&next_nodes); } if (str_idx == top_str || (cur_state && cur_state->has_backref)) { if (next_nodes.nelem) { err = expand_bkref_cache (mctx, &next_nodes, str_idx, subexp_num, type); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } } cur_state = re_acquire_state_context (&err, dfa, &next_nodes, context); if (BE (cur_state == NULL && err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } mctx->state_log[str_idx] = cur_state; } for (null_cnt = 0; str_idx < last_str && null_cnt <= mctx->max_mb_elem_len;) { re_node_set_empty (&next_nodes); if (mctx->state_log[str_idx + 1]) { err = re_node_set_merge (&next_nodes, &mctx->state_log[str_idx + 1]->nodes); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } } if (cur_state) { err = check_arrival_add_next_nodes (mctx, str_idx, &cur_state->non_eps_nodes, &next_nodes); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } } ++str_idx; if (next_nodes.nelem) { err = check_arrival_expand_ecl (dfa, &next_nodes, subexp_num, type); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } err = expand_bkref_cache (mctx, &next_nodes, str_idx, subexp_num, type); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } } context = re_string_context_at (&mctx->input, str_idx - 1, mctx->eflags); cur_state = re_acquire_state_context (&err, dfa, &next_nodes, context); if (BE (cur_state == NULL && err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } mctx->state_log[str_idx] = cur_state; null_cnt = cur_state == NULL ? null_cnt + 1 : 0; } re_node_set_free (&next_nodes); cur_nodes = (mctx->state_log[last_str] == NULL ? NULL : &mctx->state_log[last_str]->nodes); path->next_idx = str_idx; /* Fix MCTX. */ mctx->state_log = backup_state_log; mctx->input.cur_idx = backup_cur_idx; /* Then check the current node set has the node LAST_NODE. */ if (cur_nodes != NULL && re_node_set_contains (cur_nodes, last_node)) return REG_NOERROR; return REG_NOMATCH; } /* Helper functions for check_arrival. */ /* Calculate the destination nodes of CUR_NODES at STR_IDX, and append them to NEXT_NODES. TODO: This function is similar to the functions transit_state*(), however this function has many additional works. Can't we unify them? */ static reg_errcode_t internal_function __attribute_warn_unused_result__ check_arrival_add_next_nodes (re_match_context_t *mctx, Idx str_idx, re_node_set *cur_nodes, re_node_set *next_nodes) { const re_dfa_t *const dfa = mctx->dfa; bool ok; Idx cur_idx; #ifdef RE_ENABLE_I18N reg_errcode_t err = REG_NOERROR; #endif re_node_set union_set; re_node_set_init_empty (&union_set); for (cur_idx = 0; cur_idx < cur_nodes->nelem; ++cur_idx) { int naccepted = 0; Idx cur_node = cur_nodes->elems[cur_idx]; #ifdef DEBUG re_token_type_t type = dfa->nodes[cur_node].type; assert (!IS_EPSILON_NODE (type)); #endif #ifdef RE_ENABLE_I18N /* If the node may accept "multi byte". */ if (dfa->nodes[cur_node].accept_mb) { naccepted = check_node_accept_bytes (dfa, cur_node, &mctx->input, str_idx); if (naccepted > 1) { re_dfastate_t *dest_state; Idx next_node = dfa->nexts[cur_node]; Idx next_idx = str_idx + naccepted; dest_state = mctx->state_log[next_idx]; re_node_set_empty (&union_set); if (dest_state) { err = re_node_set_merge (&union_set, &dest_state->nodes); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&union_set); return err; } } ok = re_node_set_insert (&union_set, next_node); if (BE (! ok, 0)) { re_node_set_free (&union_set); return REG_ESPACE; } mctx->state_log[next_idx] = re_acquire_state (&err, dfa, &union_set); if (BE (mctx->state_log[next_idx] == NULL && err != REG_NOERROR, 0)) { re_node_set_free (&union_set); return err; } } } #endif /* RE_ENABLE_I18N */ if (naccepted || check_node_accept (mctx, dfa->nodes + cur_node, str_idx)) { ok = re_node_set_insert (next_nodes, dfa->nexts[cur_node]); if (BE (! ok, 0)) { re_node_set_free (&union_set); return REG_ESPACE; } } } re_node_set_free (&union_set); return REG_NOERROR; } /* For all the nodes in CUR_NODES, add the epsilon closures of them to CUR_NODES, however exclude the nodes which are: - inside the sub expression whose number is EX_SUBEXP, if FL_OPEN. - out of the sub expression whose number is EX_SUBEXP, if !FL_OPEN. */ static reg_errcode_t internal_function check_arrival_expand_ecl (const re_dfa_t *dfa, re_node_set *cur_nodes, Idx ex_subexp, int type) { reg_errcode_t err; Idx idx, outside_node; re_node_set new_nodes; #ifdef DEBUG assert (cur_nodes->nelem); #endif err = re_node_set_alloc (&new_nodes, cur_nodes->nelem); if (BE (err != REG_NOERROR, 0)) return err; /* Create a new node set NEW_NODES with the nodes which are epsilon closures of the node in CUR_NODES. */ for (idx = 0; idx < cur_nodes->nelem; ++idx) { Idx cur_node = cur_nodes->elems[idx]; const re_node_set *eclosure = dfa->eclosures + cur_node; outside_node = find_subexp_node (dfa, eclosure, ex_subexp, type); if (outside_node == -1) { /* There are no problematic nodes, just merge them. */ err = re_node_set_merge (&new_nodes, eclosure); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&new_nodes); return err; } } else { /* There are problematic nodes, re-calculate incrementally. */ err = check_arrival_expand_ecl_sub (dfa, &new_nodes, cur_node, ex_subexp, type); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&new_nodes); return err; } } } re_node_set_free (cur_nodes); *cur_nodes = new_nodes; return REG_NOERROR; } /* Helper function for check_arrival_expand_ecl. Check incrementally the epsilon closure of TARGET, and if it isn't problematic append it to DST_NODES. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ check_arrival_expand_ecl_sub (const re_dfa_t *dfa, re_node_set *dst_nodes, Idx target, Idx ex_subexp, int type) { Idx cur_node; for (cur_node = target; !re_node_set_contains (dst_nodes, cur_node);) { bool ok; if (dfa->nodes[cur_node].type == type && dfa->nodes[cur_node].opr.idx == ex_subexp) { if (type == OP_CLOSE_SUBEXP) { ok = re_node_set_insert (dst_nodes, cur_node); if (BE (! ok, 0)) return REG_ESPACE; } break; } ok = re_node_set_insert (dst_nodes, cur_node); if (BE (! ok, 0)) return REG_ESPACE; if (dfa->edests[cur_node].nelem == 0) break; if (dfa->edests[cur_node].nelem == 2) { reg_errcode_t err; err = check_arrival_expand_ecl_sub (dfa, dst_nodes, dfa->edests[cur_node].elems[1], ex_subexp, type); if (BE (err != REG_NOERROR, 0)) return err; } cur_node = dfa->edests[cur_node].elems[0]; } return REG_NOERROR; } /* For all the back references in the current state, calculate the destination of the back references by the appropriate entry in MCTX->BKREF_ENTS. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ expand_bkref_cache (re_match_context_t *mctx, re_node_set *cur_nodes, Idx cur_str, Idx subexp_num, int type) { const re_dfa_t *const dfa = mctx->dfa; reg_errcode_t err; Idx cache_idx_start = search_cur_bkref_entry (mctx, cur_str); struct re_backref_cache_entry *ent; if (cache_idx_start == -1) return REG_NOERROR; restart: ent = mctx->bkref_ents + cache_idx_start; do { Idx to_idx, next_node; /* Is this entry ENT is appropriate? */ if (!re_node_set_contains (cur_nodes, ent->node)) continue; /* No. */ to_idx = cur_str + ent->subexp_to - ent->subexp_from; /* Calculate the destination of the back reference, and append it to MCTX->STATE_LOG. */ if (to_idx == cur_str) { /* The backreference did epsilon transit, we must re-check all the node in the current state. */ re_node_set new_dests; reg_errcode_t err2, err3; next_node = dfa->edests[ent->node].elems[0]; if (re_node_set_contains (cur_nodes, next_node)) continue; err = re_node_set_init_1 (&new_dests, next_node); err2 = check_arrival_expand_ecl (dfa, &new_dests, subexp_num, type); err3 = re_node_set_merge (cur_nodes, &new_dests); re_node_set_free (&new_dests); if (BE (err != REG_NOERROR || err2 != REG_NOERROR || err3 != REG_NOERROR, 0)) { err = (err != REG_NOERROR ? err : (err2 != REG_NOERROR ? err2 : err3)); return err; } /* TODO: It is still inefficient... */ goto restart; } else { re_node_set union_set; next_node = dfa->nexts[ent->node]; if (mctx->state_log[to_idx]) { bool ok; if (re_node_set_contains (&mctx->state_log[to_idx]->nodes, next_node)) continue; err = re_node_set_init_copy (&union_set, &mctx->state_log[to_idx]->nodes); ok = re_node_set_insert (&union_set, next_node); if (BE (err != REG_NOERROR || ! ok, 0)) { re_node_set_free (&union_set); err = err != REG_NOERROR ? err : REG_ESPACE; return err; } } else { err = re_node_set_init_1 (&union_set, next_node); if (BE (err != REG_NOERROR, 0)) return err; } mctx->state_log[to_idx] = re_acquire_state (&err, dfa, &union_set); re_node_set_free (&union_set); if (BE (mctx->state_log[to_idx] == NULL && err != REG_NOERROR, 0)) return err; } } while (ent++->more); return REG_NOERROR; } /* Build transition table for the state. Return true if successful. */ static bool internal_function build_trtable (const re_dfa_t *dfa, re_dfastate_t *state) { reg_errcode_t err; Idx i, j; int ch; bool need_word_trtable = false; bitset_word_t elem, mask; bool dests_node_malloced = false; bool dest_states_malloced = false; Idx ndests; /* Number of the destination states from 'state'. */ re_dfastate_t **trtable; re_dfastate_t **dest_states = NULL, **dest_states_word, **dest_states_nl; re_node_set follows, *dests_node; bitset_t *dests_ch; bitset_t acceptable; struct dests_alloc { re_node_set dests_node[SBC_MAX]; bitset_t dests_ch[SBC_MAX]; } *dests_alloc; /* We build DFA states which corresponds to the destination nodes from 'state'. 'dests_node[i]' represents the nodes which i-th destination state contains, and 'dests_ch[i]' represents the characters which i-th destination state accepts. */ if (__libc_use_alloca (sizeof (struct dests_alloc))) dests_alloc = (struct dests_alloc *) alloca (sizeof (struct dests_alloc)); else { dests_alloc = re_malloc (struct dests_alloc, 1); if (BE (dests_alloc == NULL, 0)) return false; dests_node_malloced = true; } dests_node = dests_alloc->dests_node; dests_ch = dests_alloc->dests_ch; /* Initialize transition table. */ state->word_trtable = state->trtable = NULL; /* At first, group all nodes belonging to 'state' into several destinations. */ ndests = group_nodes_into_DFAstates (dfa, state, dests_node, dests_ch); if (BE (ndests <= 0, 0)) { if (dests_node_malloced) free (dests_alloc); /* Return false in case of an error, true otherwise. */ if (ndests == 0) { state->trtable = (re_dfastate_t **) calloc (sizeof (re_dfastate_t *), SBC_MAX); if (BE (state->trtable == NULL, 0)) return false; return true; } return false; } err = re_node_set_alloc (&follows, ndests + 1); if (BE (err != REG_NOERROR, 0)) goto out_free; /* Avoid arithmetic overflow in size calculation. */ if (BE ((((SIZE_MAX - (sizeof (re_node_set) + sizeof (bitset_t)) * SBC_MAX) / (3 * sizeof (re_dfastate_t *))) < ndests), 0)) goto out_free; if (__libc_use_alloca ((sizeof (re_node_set) + sizeof (bitset_t)) * SBC_MAX + ndests * 3 * sizeof (re_dfastate_t *))) dest_states = (re_dfastate_t **) alloca (ndests * 3 * sizeof (re_dfastate_t *)); else { dest_states = (re_dfastate_t **) malloc (ndests * 3 * sizeof (re_dfastate_t *)); if (BE (dest_states == NULL, 0)) { out_free: if (dest_states_malloced) free (dest_states); re_node_set_free (&follows); for (i = 0; i < ndests; ++i) re_node_set_free (dests_node + i); if (dests_node_malloced) free (dests_alloc); return false; } dest_states_malloced = true; } dest_states_word = dest_states + ndests; dest_states_nl = dest_states_word + ndests; bitset_empty (acceptable); /* Then build the states for all destinations. */ for (i = 0; i < ndests; ++i) { Idx next_node; re_node_set_empty (&follows); /* Merge the follows of this destination states. */ for (j = 0; j < dests_node[i].nelem; ++j) { next_node = dfa->nexts[dests_node[i].elems[j]]; if (next_node != -1) { err = re_node_set_merge (&follows, dfa->eclosures + next_node); if (BE (err != REG_NOERROR, 0)) goto out_free; } } dest_states[i] = re_acquire_state_context (&err, dfa, &follows, 0); if (BE (dest_states[i] == NULL && err != REG_NOERROR, 0)) goto out_free; /* If the new state has context constraint, build appropriate states for these contexts. */ if (dest_states[i]->has_constraint) { dest_states_word[i] = re_acquire_state_context (&err, dfa, &follows, CONTEXT_WORD); if (BE (dest_states_word[i] == NULL && err != REG_NOERROR, 0)) goto out_free; if (dest_states[i] != dest_states_word[i] && dfa->mb_cur_max > 1) need_word_trtable = true; dest_states_nl[i] = re_acquire_state_context (&err, dfa, &follows, CONTEXT_NEWLINE); if (BE (dest_states_nl[i] == NULL && err != REG_NOERROR, 0)) goto out_free; } else { dest_states_word[i] = dest_states[i]; dest_states_nl[i] = dest_states[i]; } bitset_merge (acceptable, dests_ch[i]); } if (!BE (need_word_trtable, 0)) { /* We don't care about whether the following character is a word character, or we are in a single-byte character set so we can discern by looking at the character code: allocate a 256-entry transition table. */ trtable = state->trtable = (re_dfastate_t **) calloc (sizeof (re_dfastate_t *), SBC_MAX); if (BE (trtable == NULL, 0)) goto out_free; /* For all characters ch...: */ for (i = 0; i < BITSET_WORDS; ++i) for (ch = i * BITSET_WORD_BITS, elem = acceptable[i], mask = 1; elem; mask <<= 1, elem >>= 1, ++ch) if (BE (elem & 1, 0)) { /* There must be exactly one destination which accepts character ch. See group_nodes_into_DFAstates. */ for (j = 0; (dests_ch[j][i] & mask) == 0; ++j) ; /* j-th destination accepts the word character ch. */ if (dfa->word_char[i] & mask) trtable[ch] = dest_states_word[j]; else trtable[ch] = dest_states[j]; } } else { /* We care about whether the following character is a word character, and we are in a multi-byte character set: discern by looking at the character code: build two 256-entry transition tables, one starting at trtable[0] and one starting at trtable[SBC_MAX]. */ trtable = state->word_trtable = (re_dfastate_t **) calloc (sizeof (re_dfastate_t *), 2 * SBC_MAX); if (BE (trtable == NULL, 0)) goto out_free; /* For all characters ch...: */ for (i = 0; i < BITSET_WORDS; ++i) for (ch = i * BITSET_WORD_BITS, elem = acceptable[i], mask = 1; elem; mask <<= 1, elem >>= 1, ++ch) if (BE (elem & 1, 0)) { /* There must be exactly one destination which accepts character ch. See group_nodes_into_DFAstates. */ for (j = 0; (dests_ch[j][i] & mask) == 0; ++j) ; /* j-th destination accepts the word character ch. */ trtable[ch] = dest_states[j]; trtable[ch + SBC_MAX] = dest_states_word[j]; } } /* new line */ if (bitset_contain (acceptable, NEWLINE_CHAR)) { /* The current state accepts newline character. */ for (j = 0; j < ndests; ++j) if (bitset_contain (dests_ch[j], NEWLINE_CHAR)) { /* k-th destination accepts newline character. */ trtable[NEWLINE_CHAR] = dest_states_nl[j]; if (need_word_trtable) trtable[NEWLINE_CHAR + SBC_MAX] = dest_states_nl[j]; /* There must be only one destination which accepts newline. See group_nodes_into_DFAstates. */ break; } } if (dest_states_malloced) free (dest_states); re_node_set_free (&follows); for (i = 0; i < ndests; ++i) re_node_set_free (dests_node + i); if (dests_node_malloced) free (dests_alloc); return true; } /* Group all nodes belonging to STATE into several destinations. Then for all destinations, set the nodes belonging to the destination to DESTS_NODE[i] and set the characters accepted by the destination to DEST_CH[i]. This function return the number of destinations. */ static Idx internal_function group_nodes_into_DFAstates (const re_dfa_t *dfa, const re_dfastate_t *state, re_node_set *dests_node, bitset_t *dests_ch) { reg_errcode_t err; bool ok; Idx i, j, k; Idx ndests; /* Number of the destinations from 'state'. */ bitset_t accepts; /* Characters a node can accept. */ const re_node_set *cur_nodes = &state->nodes; bitset_empty (accepts); ndests = 0; /* For all the nodes belonging to 'state', */ for (i = 0; i < cur_nodes->nelem; ++i) { re_token_t *node = &dfa->nodes[cur_nodes->elems[i]]; re_token_type_t type = node->type; unsigned int constraint = node->constraint; /* Enumerate all single byte character this node can accept. */ if (type == CHARACTER) bitset_set (accepts, node->opr.c); else if (type == SIMPLE_BRACKET) { bitset_merge (accepts, node->opr.sbcset); } else if (type == OP_PERIOD) { #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) bitset_merge (accepts, dfa->sb_char); else #endif bitset_set_all (accepts); if (!(dfa->syntax & RE_DOT_NEWLINE)) bitset_clear (accepts, '\n'); if (dfa->syntax & RE_DOT_NOT_NULL) bitset_clear (accepts, '\0'); } #ifdef RE_ENABLE_I18N else if (type == OP_UTF8_PERIOD) { if (ASCII_CHARS % BITSET_WORD_BITS == 0) memset (accepts, -1, ASCII_CHARS / CHAR_BIT); else bitset_merge (accepts, utf8_sb_map); if (!(dfa->syntax & RE_DOT_NEWLINE)) bitset_clear (accepts, '\n'); if (dfa->syntax & RE_DOT_NOT_NULL) bitset_clear (accepts, '\0'); } #endif else continue; /* Check the 'accepts' and sift the characters which are not match it the context. */ if (constraint) { if (constraint & NEXT_NEWLINE_CONSTRAINT) { bool accepts_newline = bitset_contain (accepts, NEWLINE_CHAR); bitset_empty (accepts); if (accepts_newline) bitset_set (accepts, NEWLINE_CHAR); else continue; } if (constraint & NEXT_ENDBUF_CONSTRAINT) { bitset_empty (accepts); continue; } if (constraint & NEXT_WORD_CONSTRAINT) { bitset_word_t any_set = 0; if (type == CHARACTER && !node->word_char) { bitset_empty (accepts); continue; } #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) for (j = 0; j < BITSET_WORDS; ++j) any_set |= (accepts[j] &= (dfa->word_char[j] | ~dfa->sb_char[j])); else #endif for (j = 0; j < BITSET_WORDS; ++j) any_set |= (accepts[j] &= dfa->word_char[j]); if (!any_set) continue; } if (constraint & NEXT_NOTWORD_CONSTRAINT) { bitset_word_t any_set = 0; if (type == CHARACTER && node->word_char) { bitset_empty (accepts); continue; } #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) for (j = 0; j < BITSET_WORDS; ++j) any_set |= (accepts[j] &= ~(dfa->word_char[j] & dfa->sb_char[j])); else #endif for (j = 0; j < BITSET_WORDS; ++j) any_set |= (accepts[j] &= ~dfa->word_char[j]); if (!any_set) continue; } } /* Then divide 'accepts' into DFA states, or create a new state. Above, we make sure that accepts is not empty. */ for (j = 0; j < ndests; ++j) { bitset_t intersec; /* Intersection sets, see below. */ bitset_t remains; /* Flags, see below. */ bitset_word_t has_intersec, not_subset, not_consumed; /* Optimization, skip if this state doesn't accept the character. */ if (type == CHARACTER && !bitset_contain (dests_ch[j], node->opr.c)) continue; /* Enumerate the intersection set of this state and 'accepts'. */ has_intersec = 0; for (k = 0; k < BITSET_WORDS; ++k) has_intersec |= intersec[k] = accepts[k] & dests_ch[j][k]; /* And skip if the intersection set is empty. */ if (!has_intersec) continue; /* Then check if this state is a subset of 'accepts'. */ not_subset = not_consumed = 0; for (k = 0; k < BITSET_WORDS; ++k) { not_subset |= remains[k] = ~accepts[k] & dests_ch[j][k]; not_consumed |= accepts[k] = accepts[k] & ~dests_ch[j][k]; } /* If this state isn't a subset of 'accepts', create a new group state, which has the 'remains'. */ if (not_subset) { bitset_copy (dests_ch[ndests], remains); bitset_copy (dests_ch[j], intersec); err = re_node_set_init_copy (dests_node + ndests, &dests_node[j]); if (BE (err != REG_NOERROR, 0)) goto error_return; ++ndests; } /* Put the position in the current group. */ ok = re_node_set_insert (&dests_node[j], cur_nodes->elems[i]); if (BE (! ok, 0)) goto error_return; /* If all characters are consumed, go to next node. */ if (!not_consumed) break; } /* Some characters remain, create a new group. */ if (j == ndests) { bitset_copy (dests_ch[ndests], accepts); err = re_node_set_init_1 (dests_node + ndests, cur_nodes->elems[i]); if (BE (err != REG_NOERROR, 0)) goto error_return; ++ndests; bitset_empty (accepts); } } return ndests; error_return: for (j = 0; j < ndests; ++j) re_node_set_free (dests_node + j); return -1; } #ifdef RE_ENABLE_I18N /* Check how many bytes the node 'dfa->nodes[node_idx]' accepts. Return the number of the bytes the node accepts. STR_IDX is the current index of the input string. This function handles the nodes which can accept one character, or one collating element like '.', '[a-z]', opposite to the other nodes can only accept one byte. */ # ifdef _LIBC # include # endif static int internal_function check_node_accept_bytes (const re_dfa_t *dfa, Idx node_idx, const re_string_t *input, Idx str_idx) { const re_token_t *node = dfa->nodes + node_idx; int char_len, elem_len; Idx i; if (BE (node->type == OP_UTF8_PERIOD, 0)) { unsigned char c = re_string_byte_at (input, str_idx), d; if (BE (c < 0xc2, 1)) return 0; if (str_idx + 2 > input->len) return 0; d = re_string_byte_at (input, str_idx + 1); if (c < 0xe0) return (d < 0x80 || d > 0xbf) ? 0 : 2; else if (c < 0xf0) { char_len = 3; if (c == 0xe0 && d < 0xa0) return 0; } else if (c < 0xf8) { char_len = 4; if (c == 0xf0 && d < 0x90) return 0; } else if (c < 0xfc) { char_len = 5; if (c == 0xf8 && d < 0x88) return 0; } else if (c < 0xfe) { char_len = 6; if (c == 0xfc && d < 0x84) return 0; } else return 0; if (str_idx + char_len > input->len) return 0; for (i = 1; i < char_len; ++i) { d = re_string_byte_at (input, str_idx + i); if (d < 0x80 || d > 0xbf) return 0; } return char_len; } char_len = re_string_char_size_at (input, str_idx); if (node->type == OP_PERIOD) { if (char_len <= 1) return 0; /* FIXME: I don't think this if is needed, as both '\n' and '\0' are char_len == 1. */ /* '.' accepts any one character except the following two cases. */ if ((!(dfa->syntax & RE_DOT_NEWLINE) && re_string_byte_at (input, str_idx) == '\n') || ((dfa->syntax & RE_DOT_NOT_NULL) && re_string_byte_at (input, str_idx) == '\0')) return 0; return char_len; } elem_len = re_string_elem_size_at (input, str_idx); if ((elem_len <= 1 && char_len <= 1) || char_len == 0) return 0; if (node->type == COMPLEX_BRACKET) { const re_charset_t *cset = node->opr.mbcset; # ifdef _LIBC const unsigned char *pin = ((const unsigned char *) re_string_get_buffer (input) + str_idx); Idx j; uint32_t nrules; # endif /* _LIBC */ int match_len = 0; wchar_t wc = ((cset->nranges || cset->nchar_classes || cset->nmbchars) ? re_string_wchar_at (input, str_idx) : 0); /* match with multibyte character? */ for (i = 0; i < cset->nmbchars; ++i) if (wc == cset->mbchars[i]) { match_len = char_len; goto check_node_accept_bytes_match; } /* match with character_class? */ for (i = 0; i < cset->nchar_classes; ++i) { wctype_t wt = cset->char_classes[i]; if (__iswctype (wc, wt)) { match_len = char_len; goto check_node_accept_bytes_match; } } # ifdef _LIBC nrules = _NL_CURRENT_WORD (LC_COLLATE, _NL_COLLATE_NRULES); if (nrules != 0) { unsigned int in_collseq = 0; const int32_t *table, *indirect; const unsigned char *weights, *extra; const char *collseqwc; /* match with collating_symbol? */ if (cset->ncoll_syms) extra = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_SYMB_EXTRAMB); for (i = 0; i < cset->ncoll_syms; ++i) { const unsigned char *coll_sym = extra + cset->coll_syms[i]; /* Compare the length of input collating element and the length of current collating element. */ if (*coll_sym != elem_len) continue; /* Compare each bytes. */ for (j = 0; j < *coll_sym; j++) if (pin[j] != coll_sym[1 + j]) break; if (j == *coll_sym) { /* Match if every bytes is equal. */ match_len = j; goto check_node_accept_bytes_match; } } if (cset->nranges) { if (elem_len <= char_len) { collseqwc = _NL_CURRENT (LC_COLLATE, _NL_COLLATE_COLLSEQWC); in_collseq = __collseq_table_lookup (collseqwc, wc); } else in_collseq = find_collation_sequence_value (pin, elem_len); } /* match with range expression? */ /* FIXME: Implement rational ranges here, too. */ for (i = 0; i < cset->nranges; ++i) if (cset->range_starts[i] <= in_collseq && in_collseq <= cset->range_ends[i]) { match_len = elem_len; goto check_node_accept_bytes_match; } /* match with equivalence_class? */ if (cset->nequiv_classes) { const unsigned char *cp = pin; table = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_TABLEMB); weights = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_WEIGHTMB); extra = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_EXTRAMB); indirect = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_INDIRECTMB); int32_t idx = findidx (table, indirect, extra, &cp, elem_len); if (idx > 0) for (i = 0; i < cset->nequiv_classes; ++i) { int32_t equiv_class_idx = cset->equiv_classes[i]; size_t weight_len = weights[idx & 0xffffff]; if (weight_len == weights[equiv_class_idx & 0xffffff] && (idx >> 24) == (equiv_class_idx >> 24)) { Idx cnt = 0; idx &= 0xffffff; equiv_class_idx &= 0xffffff; while (cnt <= weight_len && (weights[equiv_class_idx + 1 + cnt] == weights[idx + 1 + cnt])) ++cnt; if (cnt > weight_len) { match_len = elem_len; goto check_node_accept_bytes_match; } } } } } else # endif /* _LIBC */ { /* match with range expression? */ for (i = 0; i < cset->nranges; ++i) { if (cset->range_starts[i] <= wc && wc <= cset->range_ends[i]) { match_len = char_len; goto check_node_accept_bytes_match; } } } check_node_accept_bytes_match: if (!cset->non_match) return match_len; else { if (match_len > 0) return 0; else return (elem_len > char_len) ? elem_len : char_len; } } return 0; } # ifdef _LIBC static unsigned int internal_function find_collation_sequence_value (const unsigned char *mbs, size_t mbs_len) { uint32_t nrules = _NL_CURRENT_WORD (LC_COLLATE, _NL_COLLATE_NRULES); if (nrules == 0) { if (mbs_len == 1) { /* No valid character. Match it as a single byte character. */ const unsigned char *collseq = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_COLLSEQMB); return collseq[mbs[0]]; } return UINT_MAX; } else { int32_t idx; const unsigned char *extra = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_SYMB_EXTRAMB); int32_t extrasize = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_SYMB_EXTRAMB + 1) - extra; for (idx = 0; idx < extrasize;) { int mbs_cnt; bool found = false; int32_t elem_mbs_len; /* Skip the name of collating element name. */ idx = idx + extra[idx] + 1; elem_mbs_len = extra[idx++]; if (mbs_len == elem_mbs_len) { for (mbs_cnt = 0; mbs_cnt < elem_mbs_len; ++mbs_cnt) if (extra[idx + mbs_cnt] != mbs[mbs_cnt]) break; if (mbs_cnt == elem_mbs_len) /* Found the entry. */ found = true; } /* Skip the byte sequence of the collating element. */ idx += elem_mbs_len; /* Adjust for the alignment. */ idx = (idx + 3) & ~3; /* Skip the collation sequence value. */ idx += sizeof (uint32_t); /* Skip the wide char sequence of the collating element. */ idx = idx + sizeof (uint32_t) * (*(int32_t *) (extra + idx) + 1); /* If we found the entry, return the sequence value. */ if (found) return *(uint32_t *) (extra + idx); /* Skip the collation sequence value. */ idx += sizeof (uint32_t); } return UINT_MAX; } } # endif /* _LIBC */ #endif /* RE_ENABLE_I18N */ /* Check whether the node accepts the byte which is IDX-th byte of the INPUT. */ static bool internal_function check_node_accept (const re_match_context_t *mctx, const re_token_t *node, Idx idx) { unsigned char ch; ch = re_string_byte_at (&mctx->input, idx); switch (node->type) { case CHARACTER: if (node->opr.c != ch) return false; break; case SIMPLE_BRACKET: if (!bitset_contain (node->opr.sbcset, ch)) return false; break; #ifdef RE_ENABLE_I18N case OP_UTF8_PERIOD: if (ch >= ASCII_CHARS) return false; /* FALLTHROUGH */ #endif case OP_PERIOD: if ((ch == '\n' && !(mctx->dfa->syntax & RE_DOT_NEWLINE)) || (ch == '\0' && (mctx->dfa->syntax & RE_DOT_NOT_NULL))) return false; break; default: return false; } if (node->constraint) { /* The node has constraints. Check whether the current context satisfies the constraints. */ unsigned int context = re_string_context_at (&mctx->input, idx, mctx->eflags); if (NOT_SATISFY_NEXT_CONSTRAINT (node->constraint, context)) return false; } return true; } /* Extend the buffers, if the buffers have run out. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ extend_buffers (re_match_context_t *mctx, int min_len) { reg_errcode_t ret; re_string_t *pstr = &mctx->input; /* Avoid overflow. */ if (BE (MIN (IDX_MAX, SIZE_MAX / sizeof (re_dfastate_t *)) / 2 <= pstr->bufs_len, 0)) return REG_ESPACE; /* Double the lengths of the buffers, but allocate at least MIN_LEN. */ ret = re_string_realloc_buffers (pstr, MAX (min_len, MIN (pstr->len, pstr->bufs_len * 2))); if (BE (ret != REG_NOERROR, 0)) return ret; if (mctx->state_log != NULL) { /* And double the length of state_log. */ /* XXX We have no indication of the size of this buffer. If this allocation fail we have no indication that the state_log array does not have the right size. */ re_dfastate_t **new_array = re_realloc (mctx->state_log, re_dfastate_t *, pstr->bufs_len + 1); if (BE (new_array == NULL, 0)) return REG_ESPACE; mctx->state_log = new_array; } /* Then reconstruct the buffers. */ if (pstr->icase) { #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1) { ret = build_wcs_upper_buffer (pstr); if (BE (ret != REG_NOERROR, 0)) return ret; } else #endif /* RE_ENABLE_I18N */ build_upper_buffer (pstr); } else { #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1) build_wcs_buffer (pstr); else #endif /* RE_ENABLE_I18N */ { if (pstr->trans != NULL) re_string_translate_buffer (pstr); } } return REG_NOERROR; } /* Functions for matching context. */ /* Initialize MCTX. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ match_ctx_init (re_match_context_t *mctx, int eflags, Idx n) { mctx->eflags = eflags; mctx->match_last = -1; if (n > 0) { /* Avoid overflow. */ size_t max_object_size = MAX (sizeof (struct re_backref_cache_entry), sizeof (re_sub_match_top_t *)); if (BE (MIN (IDX_MAX, SIZE_MAX / max_object_size) < n, 0)) return REG_ESPACE; mctx->bkref_ents = re_malloc (struct re_backref_cache_entry, n); mctx->sub_tops = re_malloc (re_sub_match_top_t *, n); if (BE (mctx->bkref_ents == NULL || mctx->sub_tops == NULL, 0)) return REG_ESPACE; } /* Already zero-ed by the caller. else mctx->bkref_ents = NULL; mctx->nbkref_ents = 0; mctx->nsub_tops = 0; */ mctx->abkref_ents = n; mctx->max_mb_elem_len = 1; mctx->asub_tops = n; return REG_NOERROR; } /* Clean the entries which depend on the current input in MCTX. This function must be invoked when the matcher changes the start index of the input, or changes the input string. */ static void internal_function match_ctx_clean (re_match_context_t *mctx) { Idx st_idx; for (st_idx = 0; st_idx < mctx->nsub_tops; ++st_idx) { Idx sl_idx; re_sub_match_top_t *top = mctx->sub_tops[st_idx]; for (sl_idx = 0; sl_idx < top->nlasts; ++sl_idx) { re_sub_match_last_t *last = top->lasts[sl_idx]; re_free (last->path.array); re_free (last); } re_free (top->lasts); if (top->path) { re_free (top->path->array); re_free (top->path); } free (top); } mctx->nsub_tops = 0; mctx->nbkref_ents = 0; } /* Free all the memory associated with MCTX. */ static void internal_function match_ctx_free (re_match_context_t *mctx) { /* First, free all the memory associated with MCTX->SUB_TOPS. */ match_ctx_clean (mctx); re_free (mctx->sub_tops); re_free (mctx->bkref_ents); } /* Add a new backreference entry to MCTX. Note that we assume that caller never call this function with duplicate entry, and call with STR_IDX which isn't smaller than any existing entry. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ match_ctx_add_entry (re_match_context_t *mctx, Idx node, Idx str_idx, Idx from, Idx to) { if (mctx->nbkref_ents >= mctx->abkref_ents) { struct re_backref_cache_entry* new_entry; new_entry = re_realloc (mctx->bkref_ents, struct re_backref_cache_entry, mctx->abkref_ents * 2); if (BE (new_entry == NULL, 0)) { re_free (mctx->bkref_ents); return REG_ESPACE; } mctx->bkref_ents = new_entry; memset (mctx->bkref_ents + mctx->nbkref_ents, '\0', sizeof (struct re_backref_cache_entry) * mctx->abkref_ents); mctx->abkref_ents *= 2; } if (mctx->nbkref_ents > 0 && mctx->bkref_ents[mctx->nbkref_ents - 1].str_idx == str_idx) mctx->bkref_ents[mctx->nbkref_ents - 1].more = 1; mctx->bkref_ents[mctx->nbkref_ents].node = node; mctx->bkref_ents[mctx->nbkref_ents].str_idx = str_idx; mctx->bkref_ents[mctx->nbkref_ents].subexp_from = from; mctx->bkref_ents[mctx->nbkref_ents].subexp_to = to; /* This is a cache that saves negative results of check_dst_limits_calc_pos. If bit N is clear, means that this entry won't epsilon-transition to an OP_OPEN_SUBEXP or OP_CLOSE_SUBEXP for the N+1-th subexpression. If it is set, check_dst_limits_calc_pos_1 will recurse and try to find one such node. A backreference does not epsilon-transition unless it is empty, so set to all zeros if FROM != TO. */ mctx->bkref_ents[mctx->nbkref_ents].eps_reachable_subexps_map = (from == to ? -1 : 0); mctx->bkref_ents[mctx->nbkref_ents++].more = 0; if (mctx->max_mb_elem_len < to - from) mctx->max_mb_elem_len = to - from; return REG_NOERROR; } /* Return the first entry with the same str_idx, or -1 if none is found. Note that MCTX->BKREF_ENTS is already sorted by MCTX->STR_IDX. */ static Idx internal_function search_cur_bkref_entry (const re_match_context_t *mctx, Idx str_idx) { Idx left, right, mid, last; last = right = mctx->nbkref_ents; for (left = 0; left < right;) { mid = (left + right) / 2; if (mctx->bkref_ents[mid].str_idx < str_idx) left = mid + 1; else right = mid; } if (left < last && mctx->bkref_ents[left].str_idx == str_idx) return left; else return -1; } /* Register the node NODE, whose type is OP_OPEN_SUBEXP, and which matches at STR_IDX. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ match_ctx_add_subtop (re_match_context_t *mctx, Idx node, Idx str_idx) { #ifdef DEBUG assert (mctx->sub_tops != NULL); assert (mctx->asub_tops > 0); #endif if (BE (mctx->nsub_tops == mctx->asub_tops, 0)) { Idx new_asub_tops = mctx->asub_tops * 2; re_sub_match_top_t **new_array = re_realloc (mctx->sub_tops, re_sub_match_top_t *, new_asub_tops); if (BE (new_array == NULL, 0)) return REG_ESPACE; mctx->sub_tops = new_array; mctx->asub_tops = new_asub_tops; } mctx->sub_tops[mctx->nsub_tops] = calloc (1, sizeof (re_sub_match_top_t)); if (BE (mctx->sub_tops[mctx->nsub_tops] == NULL, 0)) return REG_ESPACE; mctx->sub_tops[mctx->nsub_tops]->node = node; mctx->sub_tops[mctx->nsub_tops++]->str_idx = str_idx; return REG_NOERROR; } /* Register the node NODE, whose type is OP_CLOSE_SUBEXP, and which matches at STR_IDX, whose corresponding OP_OPEN_SUBEXP is SUB_TOP. */ static re_sub_match_last_t * internal_function match_ctx_add_sublast (re_sub_match_top_t *subtop, Idx node, Idx str_idx) { re_sub_match_last_t *new_entry; if (BE (subtop->nlasts == subtop->alasts, 0)) { Idx new_alasts = 2 * subtop->alasts + 1; re_sub_match_last_t **new_array = re_realloc (subtop->lasts, re_sub_match_last_t *, new_alasts); if (BE (new_array == NULL, 0)) return NULL; subtop->lasts = new_array; subtop->alasts = new_alasts; } new_entry = calloc (1, sizeof (re_sub_match_last_t)); if (BE (new_entry != NULL, 1)) { subtop->lasts[subtop->nlasts] = new_entry; new_entry->node = node; new_entry->str_idx = str_idx; ++subtop->nlasts; } return new_entry; } static void internal_function sift_ctx_init (re_sift_context_t *sctx, re_dfastate_t **sifted_sts, re_dfastate_t **limited_sts, Idx last_node, Idx last_str_idx) { sctx->sifted_states = sifted_sts; sctx->limited_states = limited_sts; sctx->last_node = last_node; sctx->last_str_idx = last_str_idx; re_node_set_init_empty (&sctx->limits); } gnuastro-0.2.33-8a3b/bootstrapped/lib/regex_internal.c0000644000175000017500000013651113004436754017560 00000000000000/* Extended regular expression matching and search library. Copyright (C) 2002-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Contributed by Isamu Hasegawa . The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ static void re_string_construct_common (const char *str, Idx len, re_string_t *pstr, RE_TRANSLATE_TYPE trans, bool icase, const re_dfa_t *dfa) internal_function; static re_dfastate_t *create_ci_newstate (const re_dfa_t *dfa, const re_node_set *nodes, re_hashval_t hash) internal_function; static re_dfastate_t *create_cd_newstate (const re_dfa_t *dfa, const re_node_set *nodes, unsigned int context, re_hashval_t hash) internal_function; /* Functions for string operation. */ /* This function allocate the buffers. It is necessary to call re_string_reconstruct before using the object. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ re_string_allocate (re_string_t *pstr, const char *str, Idx len, Idx init_len, RE_TRANSLATE_TYPE trans, bool icase, const re_dfa_t *dfa) { reg_errcode_t ret; Idx init_buf_len; /* Ensure at least one character fits into the buffers. */ if (init_len < dfa->mb_cur_max) init_len = dfa->mb_cur_max; init_buf_len = (len + 1 < init_len) ? len + 1: init_len; re_string_construct_common (str, len, pstr, trans, icase, dfa); ret = re_string_realloc_buffers (pstr, init_buf_len); if (BE (ret != REG_NOERROR, 0)) return ret; pstr->word_char = dfa->word_char; pstr->word_ops_used = dfa->word_ops_used; pstr->mbs = pstr->mbs_allocated ? pstr->mbs : (unsigned char *) str; pstr->valid_len = (pstr->mbs_allocated || dfa->mb_cur_max > 1) ? 0 : len; pstr->valid_raw_len = pstr->valid_len; return REG_NOERROR; } /* This function allocate the buffers, and initialize them. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ re_string_construct (re_string_t *pstr, const char *str, Idx len, RE_TRANSLATE_TYPE trans, bool icase, const re_dfa_t *dfa) { reg_errcode_t ret; memset (pstr, '\0', sizeof (re_string_t)); re_string_construct_common (str, len, pstr, trans, icase, dfa); if (len > 0) { ret = re_string_realloc_buffers (pstr, len + 1); if (BE (ret != REG_NOERROR, 0)) return ret; } pstr->mbs = pstr->mbs_allocated ? pstr->mbs : (unsigned char *) str; if (icase) { #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) { while (1) { ret = build_wcs_upper_buffer (pstr); if (BE (ret != REG_NOERROR, 0)) return ret; if (pstr->valid_raw_len >= len) break; if (pstr->bufs_len > pstr->valid_len + dfa->mb_cur_max) break; ret = re_string_realloc_buffers (pstr, pstr->bufs_len * 2); if (BE (ret != REG_NOERROR, 0)) return ret; } } else #endif /* RE_ENABLE_I18N */ build_upper_buffer (pstr); } else { #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) build_wcs_buffer (pstr); else #endif /* RE_ENABLE_I18N */ { if (trans != NULL) re_string_translate_buffer (pstr); else { pstr->valid_len = pstr->bufs_len; pstr->valid_raw_len = pstr->bufs_len; } } } return REG_NOERROR; } /* Helper functions for re_string_allocate, and re_string_construct. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ re_string_realloc_buffers (re_string_t *pstr, Idx new_buf_len) { #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1) { wint_t *new_wcs; /* Avoid overflow in realloc. */ const size_t max_object_size = MAX (sizeof (wint_t), sizeof (Idx)); if (BE (MIN (IDX_MAX, SIZE_MAX / max_object_size) < new_buf_len, 0)) return REG_ESPACE; new_wcs = re_realloc (pstr->wcs, wint_t, new_buf_len); if (BE (new_wcs == NULL, 0)) return REG_ESPACE; pstr->wcs = new_wcs; if (pstr->offsets != NULL) { Idx *new_offsets = re_realloc (pstr->offsets, Idx, new_buf_len); if (BE (new_offsets == NULL, 0)) return REG_ESPACE; pstr->offsets = new_offsets; } } #endif /* RE_ENABLE_I18N */ if (pstr->mbs_allocated) { unsigned char *new_mbs = re_realloc (pstr->mbs, unsigned char, new_buf_len); if (BE (new_mbs == NULL, 0)) return REG_ESPACE; pstr->mbs = new_mbs; } pstr->bufs_len = new_buf_len; return REG_NOERROR; } static void internal_function re_string_construct_common (const char *str, Idx len, re_string_t *pstr, RE_TRANSLATE_TYPE trans, bool icase, const re_dfa_t *dfa) { pstr->raw_mbs = (const unsigned char *) str; pstr->len = len; pstr->raw_len = len; pstr->trans = trans; pstr->icase = icase; pstr->mbs_allocated = (trans != NULL || icase); pstr->mb_cur_max = dfa->mb_cur_max; pstr->is_utf8 = dfa->is_utf8; pstr->map_notascii = dfa->map_notascii; pstr->stop = pstr->len; pstr->raw_stop = pstr->stop; } #ifdef RE_ENABLE_I18N /* Build wide character buffer PSTR->WCS. If the byte sequence of the string are: (0), (1), (0), (1), Then wide character buffer will be: , WEOF , , WEOF , We use WEOF for padding, they indicate that the position isn't a first byte of a multibyte character. Note that this function assumes PSTR->VALID_LEN elements are already built and starts from PSTR->VALID_LEN. */ static void internal_function build_wcs_buffer (re_string_t *pstr) { #ifdef _LIBC unsigned char buf[MB_LEN_MAX]; assert (MB_LEN_MAX >= pstr->mb_cur_max); #else unsigned char buf[64]; #endif mbstate_t prev_st; Idx byte_idx, end_idx, remain_len; size_t mbclen; /* Build the buffers from pstr->valid_len to either pstr->len or pstr->bufs_len. */ end_idx = (pstr->bufs_len > pstr->len) ? pstr->len : pstr->bufs_len; for (byte_idx = pstr->valid_len; byte_idx < end_idx;) { wchar_t wc; const char *p; remain_len = end_idx - byte_idx; prev_st = pstr->cur_state; /* Apply the translation if we need. */ if (BE (pstr->trans != NULL, 0)) { int i, ch; for (i = 0; i < pstr->mb_cur_max && i < remain_len; ++i) { ch = pstr->raw_mbs [pstr->raw_mbs_idx + byte_idx + i]; buf[i] = pstr->mbs[byte_idx + i] = pstr->trans[ch]; } p = (const char *) buf; } else p = (const char *) pstr->raw_mbs + pstr->raw_mbs_idx + byte_idx; mbclen = __mbrtowc (&wc, p, remain_len, &pstr->cur_state); if (BE (mbclen == (size_t) -1 || mbclen == 0 || (mbclen == (size_t) -2 && pstr->bufs_len >= pstr->len), 0)) { /* We treat these cases as a singlebyte character. */ mbclen = 1; wc = (wchar_t) pstr->raw_mbs[pstr->raw_mbs_idx + byte_idx]; if (BE (pstr->trans != NULL, 0)) wc = pstr->trans[wc]; pstr->cur_state = prev_st; } else if (BE (mbclen == (size_t) -2, 0)) { /* The buffer doesn't have enough space, finish to build. */ pstr->cur_state = prev_st; break; } /* Write wide character and padding. */ pstr->wcs[byte_idx++] = wc; /* Write paddings. */ for (remain_len = byte_idx + mbclen - 1; byte_idx < remain_len ;) pstr->wcs[byte_idx++] = WEOF; } pstr->valid_len = byte_idx; pstr->valid_raw_len = byte_idx; } /* Build wide character buffer PSTR->WCS like build_wcs_buffer, but for REG_ICASE. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ build_wcs_upper_buffer (re_string_t *pstr) { mbstate_t prev_st; Idx src_idx, byte_idx, end_idx, remain_len; size_t mbclen; #ifdef _LIBC char buf[MB_LEN_MAX]; assert (MB_LEN_MAX >= pstr->mb_cur_max); #else char buf[64]; #endif byte_idx = pstr->valid_len; end_idx = (pstr->bufs_len > pstr->len) ? pstr->len : pstr->bufs_len; /* The following optimization assumes that ASCII characters can be mapped to wide characters with a simple cast. */ if (! pstr->map_notascii && pstr->trans == NULL && !pstr->offsets_needed) { while (byte_idx < end_idx) { wchar_t wc; if (isascii (pstr->raw_mbs[pstr->raw_mbs_idx + byte_idx]) && mbsinit (&pstr->cur_state)) { /* In case of a singlebyte character. */ pstr->mbs[byte_idx] = toupper (pstr->raw_mbs[pstr->raw_mbs_idx + byte_idx]); /* The next step uses the assumption that wchar_t is encoded ASCII-safe: all ASCII values can be converted like this. */ pstr->wcs[byte_idx] = (wchar_t) pstr->mbs[byte_idx]; ++byte_idx; continue; } remain_len = end_idx - byte_idx; prev_st = pstr->cur_state; mbclen = __mbrtowc (&wc, ((const char *) pstr->raw_mbs + pstr->raw_mbs_idx + byte_idx), remain_len, &pstr->cur_state); if (BE (mbclen < (size_t) -2, 1)) { wchar_t wcu = __towupper (wc); if (wcu != wc) { size_t mbcdlen; mbcdlen = __wcrtomb (buf, wcu, &prev_st); if (BE (mbclen == mbcdlen, 1)) memcpy (pstr->mbs + byte_idx, buf, mbclen); else { src_idx = byte_idx; goto offsets_needed; } } else memcpy (pstr->mbs + byte_idx, pstr->raw_mbs + pstr->raw_mbs_idx + byte_idx, mbclen); pstr->wcs[byte_idx++] = wcu; /* Write paddings. */ for (remain_len = byte_idx + mbclen - 1; byte_idx < remain_len ;) pstr->wcs[byte_idx++] = WEOF; } else if (mbclen == (size_t) -1 || mbclen == 0 || (mbclen == (size_t) -2 && pstr->bufs_len >= pstr->len)) { /* It is an invalid character, an incomplete character at the end of the string, or '\0'. Just use the byte. */ int ch = pstr->raw_mbs[pstr->raw_mbs_idx + byte_idx]; pstr->mbs[byte_idx] = ch; /* And also cast it to wide char. */ pstr->wcs[byte_idx++] = (wchar_t) ch; if (BE (mbclen == (size_t) -1, 0)) pstr->cur_state = prev_st; } else { /* The buffer doesn't have enough space, finish to build. */ pstr->cur_state = prev_st; break; } } pstr->valid_len = byte_idx; pstr->valid_raw_len = byte_idx; return REG_NOERROR; } else for (src_idx = pstr->valid_raw_len; byte_idx < end_idx;) { wchar_t wc; const char *p; offsets_needed: remain_len = end_idx - byte_idx; prev_st = pstr->cur_state; if (BE (pstr->trans != NULL, 0)) { int i, ch; for (i = 0; i < pstr->mb_cur_max && i < remain_len; ++i) { ch = pstr->raw_mbs [pstr->raw_mbs_idx + src_idx + i]; buf[i] = pstr->trans[ch]; } p = (const char *) buf; } else p = (const char *) pstr->raw_mbs + pstr->raw_mbs_idx + src_idx; mbclen = __mbrtowc (&wc, p, remain_len, &pstr->cur_state); if (BE (mbclen < (size_t) -2, 1)) { wchar_t wcu = __towupper (wc); if (wcu != wc) { size_t mbcdlen; mbcdlen = wcrtomb ((char *) buf, wcu, &prev_st); if (BE (mbclen == mbcdlen, 1)) memcpy (pstr->mbs + byte_idx, buf, mbclen); else if (mbcdlen != (size_t) -1) { size_t i; if (byte_idx + mbcdlen > pstr->bufs_len) { pstr->cur_state = prev_st; break; } if (pstr->offsets == NULL) { pstr->offsets = re_malloc (Idx, pstr->bufs_len); if (pstr->offsets == NULL) return REG_ESPACE; } if (!pstr->offsets_needed) { for (i = 0; i < (size_t) byte_idx; ++i) pstr->offsets[i] = i; pstr->offsets_needed = 1; } memcpy (pstr->mbs + byte_idx, buf, mbcdlen); pstr->wcs[byte_idx] = wcu; pstr->offsets[byte_idx] = src_idx; for (i = 1; i < mbcdlen; ++i) { pstr->offsets[byte_idx + i] = src_idx + (i < mbclen ? i : mbclen - 1); pstr->wcs[byte_idx + i] = WEOF; } pstr->len += mbcdlen - mbclen; if (pstr->raw_stop > src_idx) pstr->stop += mbcdlen - mbclen; end_idx = (pstr->bufs_len > pstr->len) ? pstr->len : pstr->bufs_len; byte_idx += mbcdlen; src_idx += mbclen; continue; } else memcpy (pstr->mbs + byte_idx, p, mbclen); } else memcpy (pstr->mbs + byte_idx, p, mbclen); if (BE (pstr->offsets_needed != 0, 0)) { size_t i; for (i = 0; i < mbclen; ++i) pstr->offsets[byte_idx + i] = src_idx + i; } src_idx += mbclen; pstr->wcs[byte_idx++] = wcu; /* Write paddings. */ for (remain_len = byte_idx + mbclen - 1; byte_idx < remain_len ;) pstr->wcs[byte_idx++] = WEOF; } else if (mbclen == (size_t) -1 || mbclen == 0 || (mbclen == (size_t) -2 && pstr->bufs_len >= pstr->len)) { /* It is an invalid character or '\0'. Just use the byte. */ int ch = pstr->raw_mbs[pstr->raw_mbs_idx + src_idx]; if (BE (pstr->trans != NULL, 0)) ch = pstr->trans [ch]; pstr->mbs[byte_idx] = ch; if (BE (pstr->offsets_needed != 0, 0)) pstr->offsets[byte_idx] = src_idx; ++src_idx; /* And also cast it to wide char. */ pstr->wcs[byte_idx++] = (wchar_t) ch; if (BE (mbclen == (size_t) -1, 0)) pstr->cur_state = prev_st; } else { /* The buffer doesn't have enough space, finish to build. */ pstr->cur_state = prev_st; break; } } pstr->valid_len = byte_idx; pstr->valid_raw_len = src_idx; return REG_NOERROR; } /* Skip characters until the index becomes greater than NEW_RAW_IDX. Return the index. */ static Idx internal_function re_string_skip_chars (re_string_t *pstr, Idx new_raw_idx, wint_t *last_wc) { mbstate_t prev_st; Idx rawbuf_idx; size_t mbclen; wint_t wc = WEOF; /* Skip the characters which are not necessary to check. */ for (rawbuf_idx = pstr->raw_mbs_idx + pstr->valid_raw_len; rawbuf_idx < new_raw_idx;) { wchar_t wc2; Idx remain_len = pstr->raw_len - rawbuf_idx; prev_st = pstr->cur_state; mbclen = __mbrtowc (&wc2, (const char *) pstr->raw_mbs + rawbuf_idx, remain_len, &pstr->cur_state); if (BE (mbclen == (size_t) -2 || mbclen == (size_t) -1 || mbclen == 0, 0)) { /* We treat these cases as a single byte character. */ if (mbclen == 0 || remain_len == 0) wc = L'\0'; else wc = *(unsigned char *) (pstr->raw_mbs + rawbuf_idx); mbclen = 1; pstr->cur_state = prev_st; } else wc = wc2; /* Then proceed the next character. */ rawbuf_idx += mbclen; } *last_wc = wc; return rawbuf_idx; } #endif /* RE_ENABLE_I18N */ /* Build the buffer PSTR->MBS, and apply the translation if we need. This function is used in case of REG_ICASE. */ static void internal_function build_upper_buffer (re_string_t *pstr) { Idx char_idx, end_idx; end_idx = (pstr->bufs_len > pstr->len) ? pstr->len : pstr->bufs_len; for (char_idx = pstr->valid_len; char_idx < end_idx; ++char_idx) { int ch = pstr->raw_mbs[pstr->raw_mbs_idx + char_idx]; if (BE (pstr->trans != NULL, 0)) ch = pstr->trans[ch]; pstr->mbs[char_idx] = toupper (ch); } pstr->valid_len = char_idx; pstr->valid_raw_len = char_idx; } /* Apply TRANS to the buffer in PSTR. */ static void internal_function re_string_translate_buffer (re_string_t *pstr) { Idx buf_idx, end_idx; end_idx = (pstr->bufs_len > pstr->len) ? pstr->len : pstr->bufs_len; for (buf_idx = pstr->valid_len; buf_idx < end_idx; ++buf_idx) { int ch = pstr->raw_mbs[pstr->raw_mbs_idx + buf_idx]; pstr->mbs[buf_idx] = pstr->trans[ch]; } pstr->valid_len = buf_idx; pstr->valid_raw_len = buf_idx; } /* This function re-construct the buffers. Concretely, convert to wide character in case of pstr->mb_cur_max > 1, convert to upper case in case of REG_ICASE, apply translation. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ re_string_reconstruct (re_string_t *pstr, Idx idx, int eflags) { Idx offset; if (BE (pstr->raw_mbs_idx <= idx, 0)) offset = idx - pstr->raw_mbs_idx; else { /* Reset buffer. */ #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1) memset (&pstr->cur_state, '\0', sizeof (mbstate_t)); #endif /* RE_ENABLE_I18N */ pstr->len = pstr->raw_len; pstr->stop = pstr->raw_stop; pstr->valid_len = 0; pstr->raw_mbs_idx = 0; pstr->valid_raw_len = 0; pstr->offsets_needed = 0; pstr->tip_context = ((eflags & REG_NOTBOL) ? CONTEXT_BEGBUF : CONTEXT_NEWLINE | CONTEXT_BEGBUF); if (!pstr->mbs_allocated) pstr->mbs = (unsigned char *) pstr->raw_mbs; offset = idx; } if (BE (offset != 0, 1)) { /* Should the already checked characters be kept? */ if (BE (offset < pstr->valid_raw_len, 1)) { /* Yes, move them to the front of the buffer. */ #ifdef RE_ENABLE_I18N if (BE (pstr->offsets_needed, 0)) { Idx low = 0, high = pstr->valid_len, mid; do { mid = (high + low) / 2; if (pstr->offsets[mid] > offset) high = mid; else if (pstr->offsets[mid] < offset) low = mid + 1; else break; } while (low < high); if (pstr->offsets[mid] < offset) ++mid; pstr->tip_context = re_string_context_at (pstr, mid - 1, eflags); /* This can be quite complicated, so handle specially only the common and easy case where the character with different length representation of lower and upper case is present at or after offset. */ if (pstr->valid_len > offset && mid == offset && pstr->offsets[mid] == offset) { memmove (pstr->wcs, pstr->wcs + offset, (pstr->valid_len - offset) * sizeof (wint_t)); memmove (pstr->mbs, pstr->mbs + offset, pstr->valid_len - offset); pstr->valid_len -= offset; pstr->valid_raw_len -= offset; for (low = 0; low < pstr->valid_len; low++) pstr->offsets[low] = pstr->offsets[low + offset] - offset; } else { /* Otherwise, just find out how long the partial multibyte character at offset is and fill it with WEOF/255. */ pstr->len = pstr->raw_len - idx + offset; pstr->stop = pstr->raw_stop - idx + offset; pstr->offsets_needed = 0; while (mid > 0 && pstr->offsets[mid - 1] == offset) --mid; while (mid < pstr->valid_len) if (pstr->wcs[mid] != WEOF) break; else ++mid; if (mid == pstr->valid_len) pstr->valid_len = 0; else { pstr->valid_len = pstr->offsets[mid] - offset; if (pstr->valid_len) { for (low = 0; low < pstr->valid_len; ++low) pstr->wcs[low] = WEOF; memset (pstr->mbs, 255, pstr->valid_len); } } pstr->valid_raw_len = pstr->valid_len; } } else #endif { pstr->tip_context = re_string_context_at (pstr, offset - 1, eflags); #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1) memmove (pstr->wcs, pstr->wcs + offset, (pstr->valid_len - offset) * sizeof (wint_t)); #endif /* RE_ENABLE_I18N */ if (BE (pstr->mbs_allocated, 0)) memmove (pstr->mbs, pstr->mbs + offset, pstr->valid_len - offset); pstr->valid_len -= offset; pstr->valid_raw_len -= offset; #if defined DEBUG && DEBUG assert (pstr->valid_len > 0); #endif } } else { #ifdef RE_ENABLE_I18N /* No, skip all characters until IDX. */ Idx prev_valid_len = pstr->valid_len; if (BE (pstr->offsets_needed, 0)) { pstr->len = pstr->raw_len - idx + offset; pstr->stop = pstr->raw_stop - idx + offset; pstr->offsets_needed = 0; } #endif pstr->valid_len = 0; #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1) { Idx wcs_idx; wint_t wc = WEOF; if (pstr->is_utf8) { const unsigned char *raw, *p, *end; /* Special case UTF-8. Multi-byte chars start with any byte other than 0x80 - 0xbf. */ raw = pstr->raw_mbs + pstr->raw_mbs_idx; end = raw + (offset - pstr->mb_cur_max); if (end < pstr->raw_mbs) end = pstr->raw_mbs; p = raw + offset - 1; #ifdef _LIBC /* We know the wchar_t encoding is UCS4, so for the simple case, ASCII characters, skip the conversion step. */ if (isascii (*p) && BE (pstr->trans == NULL, 1)) { memset (&pstr->cur_state, '\0', sizeof (mbstate_t)); /* pstr->valid_len = 0; */ wc = (wchar_t) *p; } else #endif for (; p >= end; --p) if ((*p & 0xc0) != 0x80) { mbstate_t cur_state; wchar_t wc2; Idx mlen = raw + pstr->len - p; unsigned char buf[6]; size_t mbclen; const unsigned char *pp = p; if (BE (pstr->trans != NULL, 0)) { int i = mlen < 6 ? mlen : 6; while (--i >= 0) buf[i] = pstr->trans[p[i]]; pp = buf; } /* XXX Don't use mbrtowc, we know which conversion to use (UTF-8 -> UCS4). */ memset (&cur_state, 0, sizeof (cur_state)); mbclen = __mbrtowc (&wc2, (const char *) pp, mlen, &cur_state); if (raw + offset - p <= mbclen && mbclen < (size_t) -2) { memset (&pstr->cur_state, '\0', sizeof (mbstate_t)); pstr->valid_len = mbclen - (raw + offset - p); wc = wc2; } break; } } if (wc == WEOF) pstr->valid_len = re_string_skip_chars (pstr, idx, &wc) - idx; if (wc == WEOF) pstr->tip_context = re_string_context_at (pstr, prev_valid_len - 1, eflags); else pstr->tip_context = ((BE (pstr->word_ops_used != 0, 0) && IS_WIDE_WORD_CHAR (wc)) ? CONTEXT_WORD : ((IS_WIDE_NEWLINE (wc) && pstr->newline_anchor) ? CONTEXT_NEWLINE : 0)); if (BE (pstr->valid_len, 0)) { for (wcs_idx = 0; wcs_idx < pstr->valid_len; ++wcs_idx) pstr->wcs[wcs_idx] = WEOF; if (pstr->mbs_allocated) memset (pstr->mbs, 255, pstr->valid_len); } pstr->valid_raw_len = pstr->valid_len; } else #endif /* RE_ENABLE_I18N */ { int c = pstr->raw_mbs[pstr->raw_mbs_idx + offset - 1]; pstr->valid_raw_len = 0; if (pstr->trans) c = pstr->trans[c]; pstr->tip_context = (bitset_contain (pstr->word_char, c) ? CONTEXT_WORD : ((IS_NEWLINE (c) && pstr->newline_anchor) ? CONTEXT_NEWLINE : 0)); } } if (!BE (pstr->mbs_allocated, 0)) pstr->mbs += offset; } pstr->raw_mbs_idx = idx; pstr->len -= offset; pstr->stop -= offset; /* Then build the buffers. */ #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1) { if (pstr->icase) { reg_errcode_t ret = build_wcs_upper_buffer (pstr); if (BE (ret != REG_NOERROR, 0)) return ret; } else build_wcs_buffer (pstr); } else #endif /* RE_ENABLE_I18N */ if (BE (pstr->mbs_allocated, 0)) { if (pstr->icase) build_upper_buffer (pstr); else if (pstr->trans != NULL) re_string_translate_buffer (pstr); } else pstr->valid_len = pstr->len; pstr->cur_idx = 0; return REG_NOERROR; } static unsigned char internal_function __attribute__ ((pure)) re_string_peek_byte_case (const re_string_t *pstr, Idx idx) { int ch; Idx off; /* Handle the common (easiest) cases first. */ if (BE (!pstr->mbs_allocated, 1)) return re_string_peek_byte (pstr, idx); #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1 && ! re_string_is_single_byte_char (pstr, pstr->cur_idx + idx)) return re_string_peek_byte (pstr, idx); #endif off = pstr->cur_idx + idx; #ifdef RE_ENABLE_I18N if (pstr->offsets_needed) off = pstr->offsets[off]; #endif ch = pstr->raw_mbs[pstr->raw_mbs_idx + off]; #ifdef RE_ENABLE_I18N /* Ensure that e.g. for tr_TR.UTF-8 BACKSLASH DOTLESS SMALL LETTER I this function returns CAPITAL LETTER I instead of first byte of DOTLESS SMALL LETTER I. The latter would confuse the parser, since peek_byte_case doesn't advance cur_idx in any way. */ if (pstr->offsets_needed && !isascii (ch)) return re_string_peek_byte (pstr, idx); #endif return ch; } static unsigned char internal_function re_string_fetch_byte_case (re_string_t *pstr) { if (BE (!pstr->mbs_allocated, 1)) return re_string_fetch_byte (pstr); #ifdef RE_ENABLE_I18N if (pstr->offsets_needed) { Idx off; int ch; /* For tr_TR.UTF-8 [[:islower:]] there is [[: CAPITAL LETTER I WITH DOT lower:]] in mbs. Skip in that case the whole multi-byte character and return the original letter. On the other side, with [[: DOTLESS SMALL LETTER I return [[:I, as doing anything else would complicate things too much. */ if (!re_string_first_byte (pstr, pstr->cur_idx)) return re_string_fetch_byte (pstr); off = pstr->offsets[pstr->cur_idx]; ch = pstr->raw_mbs[pstr->raw_mbs_idx + off]; if (! isascii (ch)) return re_string_fetch_byte (pstr); re_string_skip_bytes (pstr, re_string_char_size_at (pstr, pstr->cur_idx)); return ch; } #endif return pstr->raw_mbs[pstr->raw_mbs_idx + pstr->cur_idx++]; } static void internal_function re_string_destruct (re_string_t *pstr) { #ifdef RE_ENABLE_I18N re_free (pstr->wcs); re_free (pstr->offsets); #endif /* RE_ENABLE_I18N */ if (pstr->mbs_allocated) re_free (pstr->mbs); } /* Return the context at IDX in INPUT. */ static unsigned int internal_function re_string_context_at (const re_string_t *input, Idx idx, int eflags) { int c; if (BE (idx < 0, 0)) /* In this case, we use the value stored in input->tip_context, since we can't know the character in input->mbs[-1] here. */ return input->tip_context; if (BE (idx == input->len, 0)) return ((eflags & REG_NOTEOL) ? CONTEXT_ENDBUF : CONTEXT_NEWLINE | CONTEXT_ENDBUF); #ifdef RE_ENABLE_I18N if (input->mb_cur_max > 1) { wint_t wc; Idx wc_idx = idx; while(input->wcs[wc_idx] == WEOF) { #if defined DEBUG && DEBUG /* It must not happen. */ assert (wc_idx >= 0); #endif --wc_idx; if (wc_idx < 0) return input->tip_context; } wc = input->wcs[wc_idx]; if (BE (input->word_ops_used != 0, 0) && IS_WIDE_WORD_CHAR (wc)) return CONTEXT_WORD; return (IS_WIDE_NEWLINE (wc) && input->newline_anchor ? CONTEXT_NEWLINE : 0); } else #endif { c = re_string_byte_at (input, idx); if (bitset_contain (input->word_char, c)) return CONTEXT_WORD; return IS_NEWLINE (c) && input->newline_anchor ? CONTEXT_NEWLINE : 0; } } /* Functions for set operation. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ re_node_set_alloc (re_node_set *set, Idx size) { set->alloc = size; set->nelem = 0; set->elems = re_malloc (Idx, size); if (BE (set->elems == NULL, 0) && (MALLOC_0_IS_NONNULL || size != 0)) return REG_ESPACE; return REG_NOERROR; } static reg_errcode_t internal_function __attribute_warn_unused_result__ re_node_set_init_1 (re_node_set *set, Idx elem) { set->alloc = 1; set->nelem = 1; set->elems = re_malloc (Idx, 1); if (BE (set->elems == NULL, 0)) { set->alloc = set->nelem = 0; return REG_ESPACE; } set->elems[0] = elem; return REG_NOERROR; } static reg_errcode_t internal_function __attribute_warn_unused_result__ re_node_set_init_2 (re_node_set *set, Idx elem1, Idx elem2) { set->alloc = 2; set->elems = re_malloc (Idx, 2); if (BE (set->elems == NULL, 0)) return REG_ESPACE; if (elem1 == elem2) { set->nelem = 1; set->elems[0] = elem1; } else { set->nelem = 2; if (elem1 < elem2) { set->elems[0] = elem1; set->elems[1] = elem2; } else { set->elems[0] = elem2; set->elems[1] = elem1; } } return REG_NOERROR; } static reg_errcode_t internal_function __attribute_warn_unused_result__ re_node_set_init_copy (re_node_set *dest, const re_node_set *src) { dest->nelem = src->nelem; if (src->nelem > 0) { dest->alloc = dest->nelem; dest->elems = re_malloc (Idx, dest->alloc); if (BE (dest->elems == NULL, 0)) { dest->alloc = dest->nelem = 0; return REG_ESPACE; } memcpy (dest->elems, src->elems, src->nelem * sizeof (Idx)); } else re_node_set_init_empty (dest); return REG_NOERROR; } /* Calculate the intersection of the sets SRC1 and SRC2. And merge it to DEST. Return value indicate the error code or REG_NOERROR if succeeded. Note: We assume dest->elems is NULL, when dest->alloc is 0. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ re_node_set_add_intersect (re_node_set *dest, const re_node_set *src1, const re_node_set *src2) { Idx i1, i2, is, id, delta, sbase; if (src1->nelem == 0 || src2->nelem == 0) return REG_NOERROR; /* We need dest->nelem + 2 * elems_in_intersection; this is a conservative estimate. */ if (src1->nelem + src2->nelem + dest->nelem > dest->alloc) { Idx new_alloc = src1->nelem + src2->nelem + dest->alloc; Idx *new_elems = re_realloc (dest->elems, Idx, new_alloc); if (BE (new_elems == NULL, 0)) return REG_ESPACE; dest->elems = new_elems; dest->alloc = new_alloc; } /* Find the items in the intersection of SRC1 and SRC2, and copy into the top of DEST those that are not already in DEST itself. */ sbase = dest->nelem + src1->nelem + src2->nelem; i1 = src1->nelem - 1; i2 = src2->nelem - 1; id = dest->nelem - 1; for (;;) { if (src1->elems[i1] == src2->elems[i2]) { /* Try to find the item in DEST. Maybe we could binary search? */ while (id >= 0 && dest->elems[id] > src1->elems[i1]) --id; if (id < 0 || dest->elems[id] != src1->elems[i1]) dest->elems[--sbase] = src1->elems[i1]; if (--i1 < 0 || --i2 < 0) break; } /* Lower the highest of the two items. */ else if (src1->elems[i1] < src2->elems[i2]) { if (--i2 < 0) break; } else { if (--i1 < 0) break; } } id = dest->nelem - 1; is = dest->nelem + src1->nelem + src2->nelem - 1; delta = is - sbase + 1; /* Now copy. When DELTA becomes zero, the remaining DEST elements are already in place; this is more or less the same loop that is in re_node_set_merge. */ dest->nelem += delta; if (delta > 0 && id >= 0) for (;;) { if (dest->elems[is] > dest->elems[id]) { /* Copy from the top. */ dest->elems[id + delta--] = dest->elems[is--]; if (delta == 0) break; } else { /* Slide from the bottom. */ dest->elems[id + delta] = dest->elems[id]; if (--id < 0) break; } } /* Copy remaining SRC elements. */ memcpy (dest->elems, dest->elems + sbase, delta * sizeof (Idx)); return REG_NOERROR; } /* Calculate the union set of the sets SRC1 and SRC2. And store it to DEST. Return value indicate the error code or REG_NOERROR if succeeded. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ re_node_set_init_union (re_node_set *dest, const re_node_set *src1, const re_node_set *src2) { Idx i1, i2, id; if (src1 != NULL && src1->nelem > 0 && src2 != NULL && src2->nelem > 0) { dest->alloc = src1->nelem + src2->nelem; dest->elems = re_malloc (Idx, dest->alloc); if (BE (dest->elems == NULL, 0)) return REG_ESPACE; } else { if (src1 != NULL && src1->nelem > 0) return re_node_set_init_copy (dest, src1); else if (src2 != NULL && src2->nelem > 0) return re_node_set_init_copy (dest, src2); else re_node_set_init_empty (dest); return REG_NOERROR; } for (i1 = i2 = id = 0 ; i1 < src1->nelem && i2 < src2->nelem ;) { if (src1->elems[i1] > src2->elems[i2]) { dest->elems[id++] = src2->elems[i2++]; continue; } if (src1->elems[i1] == src2->elems[i2]) ++i2; dest->elems[id++] = src1->elems[i1++]; } if (i1 < src1->nelem) { memcpy (dest->elems + id, src1->elems + i1, (src1->nelem - i1) * sizeof (Idx)); id += src1->nelem - i1; } else if (i2 < src2->nelem) { memcpy (dest->elems + id, src2->elems + i2, (src2->nelem - i2) * sizeof (Idx)); id += src2->nelem - i2; } dest->nelem = id; return REG_NOERROR; } /* Calculate the union set of the sets DEST and SRC. And store it to DEST. Return value indicate the error code or REG_NOERROR if succeeded. */ static reg_errcode_t internal_function __attribute_warn_unused_result__ re_node_set_merge (re_node_set *dest, const re_node_set *src) { Idx is, id, sbase, delta; if (src == NULL || src->nelem == 0) return REG_NOERROR; if (dest->alloc < 2 * src->nelem + dest->nelem) { Idx new_alloc = 2 * (src->nelem + dest->alloc); Idx *new_buffer = re_realloc (dest->elems, Idx, new_alloc); if (BE (new_buffer == NULL, 0)) return REG_ESPACE; dest->elems = new_buffer; dest->alloc = new_alloc; } if (BE (dest->nelem == 0, 0)) { dest->nelem = src->nelem; memcpy (dest->elems, src->elems, src->nelem * sizeof (Idx)); return REG_NOERROR; } /* Copy into the top of DEST the items of SRC that are not found in DEST. Maybe we could binary search in DEST? */ for (sbase = dest->nelem + 2 * src->nelem, is = src->nelem - 1, id = dest->nelem - 1; is >= 0 && id >= 0; ) { if (dest->elems[id] == src->elems[is]) is--, id--; else if (dest->elems[id] < src->elems[is]) dest->elems[--sbase] = src->elems[is--]; else /* if (dest->elems[id] > src->elems[is]) */ --id; } if (is >= 0) { /* If DEST is exhausted, the remaining items of SRC must be unique. */ sbase -= is + 1; memcpy (dest->elems + sbase, src->elems, (is + 1) * sizeof (Idx)); } id = dest->nelem - 1; is = dest->nelem + 2 * src->nelem - 1; delta = is - sbase + 1; if (delta == 0) return REG_NOERROR; /* Now copy. When DELTA becomes zero, the remaining DEST elements are already in place. */ dest->nelem += delta; for (;;) { if (dest->elems[is] > dest->elems[id]) { /* Copy from the top. */ dest->elems[id + delta--] = dest->elems[is--]; if (delta == 0) break; } else { /* Slide from the bottom. */ dest->elems[id + delta] = dest->elems[id]; if (--id < 0) { /* Copy remaining SRC elements. */ memcpy (dest->elems, dest->elems + sbase, delta * sizeof (Idx)); break; } } } return REG_NOERROR; } /* Insert the new element ELEM to the re_node_set* SET. SET should not already have ELEM. Return true if successful. */ static bool internal_function __attribute_warn_unused_result__ re_node_set_insert (re_node_set *set, Idx elem) { Idx idx; /* In case the set is empty. */ if (set->alloc == 0) return BE (re_node_set_init_1 (set, elem) == REG_NOERROR, 1); if (BE (set->nelem, 0) == 0) { /* We already guaranteed above that set->alloc != 0. */ set->elems[0] = elem; ++set->nelem; return true; } /* Realloc if we need. */ if (set->alloc == set->nelem) { Idx *new_elems; set->alloc = set->alloc * 2; new_elems = re_realloc (set->elems, Idx, set->alloc); if (BE (new_elems == NULL, 0)) return false; set->elems = new_elems; } /* Move the elements which follows the new element. Test the first element separately to skip a check in the inner loop. */ if (elem < set->elems[0]) { idx = 0; for (idx = set->nelem; idx > 0; idx--) set->elems[idx] = set->elems[idx - 1]; } else { for (idx = set->nelem; set->elems[idx - 1] > elem; idx--) set->elems[idx] = set->elems[idx - 1]; } /* Insert the new element. */ set->elems[idx] = elem; ++set->nelem; return true; } /* Insert the new element ELEM to the re_node_set* SET. SET should not already have any element greater than or equal to ELEM. Return true if successful. */ static bool internal_function __attribute_warn_unused_result__ re_node_set_insert_last (re_node_set *set, Idx elem) { /* Realloc if we need. */ if (set->alloc == set->nelem) { Idx *new_elems; set->alloc = (set->alloc + 1) * 2; new_elems = re_realloc (set->elems, Idx, set->alloc); if (BE (new_elems == NULL, 0)) return false; set->elems = new_elems; } /* Insert the new element. */ set->elems[set->nelem++] = elem; return true; } /* Compare two node sets SET1 and SET2. Return true if SET1 and SET2 are equivalent. */ static bool internal_function __attribute__ ((pure)) re_node_set_compare (const re_node_set *set1, const re_node_set *set2) { Idx i; if (set1 == NULL || set2 == NULL || set1->nelem != set2->nelem) return false; for (i = set1->nelem ; --i >= 0 ; ) if (set1->elems[i] != set2->elems[i]) return false; return true; } /* Return (idx + 1) if SET contains the element ELEM, return 0 otherwise. */ static Idx internal_function __attribute__ ((pure)) re_node_set_contains (const re_node_set *set, Idx elem) { __re_size_t idx, right, mid; if (set->nelem <= 0) return 0; /* Binary search the element. */ idx = 0; right = set->nelem - 1; while (idx < right) { mid = (idx + right) / 2; if (set->elems[mid] < elem) idx = mid + 1; else right = mid; } return set->elems[idx] == elem ? idx + 1 : 0; } static void internal_function re_node_set_remove_at (re_node_set *set, Idx idx) { if (idx < 0 || idx >= set->nelem) return; --set->nelem; for (; idx < set->nelem; idx++) set->elems[idx] = set->elems[idx + 1]; } /* Add the token TOKEN to dfa->nodes, and return the index of the token. Or return -1 if an error occurred. */ static Idx internal_function re_dfa_add_node (re_dfa_t *dfa, re_token_t token) { if (BE (dfa->nodes_len >= dfa->nodes_alloc, 0)) { size_t new_nodes_alloc = dfa->nodes_alloc * 2; Idx *new_nexts, *new_indices; re_node_set *new_edests, *new_eclosures; re_token_t *new_nodes; /* Avoid overflows in realloc. */ const size_t max_object_size = MAX (sizeof (re_token_t), MAX (sizeof (re_node_set), sizeof (Idx))); if (BE (MIN (IDX_MAX, SIZE_MAX / max_object_size) < new_nodes_alloc, 0)) return -1; new_nodes = re_realloc (dfa->nodes, re_token_t, new_nodes_alloc); if (BE (new_nodes == NULL, 0)) return -1; dfa->nodes = new_nodes; new_nexts = re_realloc (dfa->nexts, Idx, new_nodes_alloc); new_indices = re_realloc (dfa->org_indices, Idx, new_nodes_alloc); new_edests = re_realloc (dfa->edests, re_node_set, new_nodes_alloc); new_eclosures = re_realloc (dfa->eclosures, re_node_set, new_nodes_alloc); if (BE (new_nexts == NULL || new_indices == NULL || new_edests == NULL || new_eclosures == NULL, 0)) { re_free (new_nexts); re_free (new_indices); re_free (new_edests); re_free (new_eclosures); return -1; } dfa->nexts = new_nexts; dfa->org_indices = new_indices; dfa->edests = new_edests; dfa->eclosures = new_eclosures; dfa->nodes_alloc = new_nodes_alloc; } dfa->nodes[dfa->nodes_len] = token; dfa->nodes[dfa->nodes_len].constraint = 0; #ifdef RE_ENABLE_I18N dfa->nodes[dfa->nodes_len].accept_mb = ((token.type == OP_PERIOD && dfa->mb_cur_max > 1) || token.type == COMPLEX_BRACKET); #endif dfa->nexts[dfa->nodes_len] = -1; re_node_set_init_empty (dfa->edests + dfa->nodes_len); re_node_set_init_empty (dfa->eclosures + dfa->nodes_len); return dfa->nodes_len++; } static re_hashval_t internal_function calc_state_hash (const re_node_set *nodes, unsigned int context) { re_hashval_t hash = nodes->nelem + context; Idx i; for (i = 0 ; i < nodes->nelem ; i++) hash += nodes->elems[i]; return hash; } /* Search for the state whose node_set is equivalent to NODES. Return the pointer to the state, if we found it in the DFA. Otherwise create the new one and return it. In case of an error return NULL and set the error code in ERR. Note: - We assume NULL as the invalid state, then it is possible that return value is NULL and ERR is REG_NOERROR. - We never return non-NULL value in case of any errors, it is for optimization. */ static re_dfastate_t * internal_function __attribute_warn_unused_result__ re_acquire_state (reg_errcode_t *err, const re_dfa_t *dfa, const re_node_set *nodes) { re_hashval_t hash; re_dfastate_t *new_state; struct re_state_table_entry *spot; Idx i; #if defined GCC_LINT || defined lint /* Suppress bogus uninitialized-variable warnings. */ *err = REG_NOERROR; #endif if (BE (nodes->nelem == 0, 0)) { *err = REG_NOERROR; return NULL; } hash = calc_state_hash (nodes, 0); spot = dfa->state_table + (hash & dfa->state_hash_mask); for (i = 0 ; i < spot->num ; i++) { re_dfastate_t *state = spot->array[i]; if (hash != state->hash) continue; if (re_node_set_compare (&state->nodes, nodes)) return state; } /* There are no appropriate state in the dfa, create the new one. */ new_state = create_ci_newstate (dfa, nodes, hash); if (BE (new_state == NULL, 0)) *err = REG_ESPACE; return new_state; } /* Search for the state whose node_set is equivalent to NODES and whose context is equivalent to CONTEXT. Return the pointer to the state, if we found it in the DFA. Otherwise create the new one and return it. In case of an error return NULL and set the error code in ERR. Note: - We assume NULL as the invalid state, then it is possible that return value is NULL and ERR is REG_NOERROR. - We never return non-NULL value in case of any errors, it is for optimization. */ static re_dfastate_t * internal_function __attribute_warn_unused_result__ re_acquire_state_context (reg_errcode_t *err, const re_dfa_t *dfa, const re_node_set *nodes, unsigned int context) { re_hashval_t hash; re_dfastate_t *new_state; struct re_state_table_entry *spot; Idx i; #if defined GCC_LINT || defined lint /* Suppress bogus uninitialized-variable warnings. */ *err = REG_NOERROR; #endif if (nodes->nelem == 0) { *err = REG_NOERROR; return NULL; } hash = calc_state_hash (nodes, context); spot = dfa->state_table + (hash & dfa->state_hash_mask); for (i = 0 ; i < spot->num ; i++) { re_dfastate_t *state = spot->array[i]; if (state->hash == hash && state->context == context && re_node_set_compare (state->entrance_nodes, nodes)) return state; } /* There are no appropriate state in 'dfa', create the new one. */ new_state = create_cd_newstate (dfa, nodes, context, hash); if (BE (new_state == NULL, 0)) *err = REG_ESPACE; return new_state; } /* Finish initialization of the new state NEWSTATE, and using its hash value HASH put in the appropriate bucket of DFA's state table. Return value indicates the error code if failed. */ static reg_errcode_t __attribute_warn_unused_result__ register_state (const re_dfa_t *dfa, re_dfastate_t *newstate, re_hashval_t hash) { struct re_state_table_entry *spot; reg_errcode_t err; Idx i; newstate->hash = hash; err = re_node_set_alloc (&newstate->non_eps_nodes, newstate->nodes.nelem); if (BE (err != REG_NOERROR, 0)) return REG_ESPACE; for (i = 0; i < newstate->nodes.nelem; i++) { Idx elem = newstate->nodes.elems[i]; if (!IS_EPSILON_NODE (dfa->nodes[elem].type)) if (! re_node_set_insert_last (&newstate->non_eps_nodes, elem)) return REG_ESPACE; } spot = dfa->state_table + (hash & dfa->state_hash_mask); if (BE (spot->alloc <= spot->num, 0)) { Idx new_alloc = 2 * spot->num + 2; re_dfastate_t **new_array = re_realloc (spot->array, re_dfastate_t *, new_alloc); if (BE (new_array == NULL, 0)) return REG_ESPACE; spot->array = new_array; spot->alloc = new_alloc; } spot->array[spot->num++] = newstate; return REG_NOERROR; } static void free_state (re_dfastate_t *state) { re_node_set_free (&state->non_eps_nodes); re_node_set_free (&state->inveclosure); if (state->entrance_nodes != &state->nodes) { re_node_set_free (state->entrance_nodes); re_free (state->entrance_nodes); } re_node_set_free (&state->nodes); re_free (state->word_trtable); re_free (state->trtable); re_free (state); } /* Create the new state which is independent of contexts. Return the new state if succeeded, otherwise return NULL. */ static re_dfastate_t * internal_function __attribute_warn_unused_result__ create_ci_newstate (const re_dfa_t *dfa, const re_node_set *nodes, re_hashval_t hash) { Idx i; reg_errcode_t err; re_dfastate_t *newstate; newstate = (re_dfastate_t *) calloc (sizeof (re_dfastate_t), 1); if (BE (newstate == NULL, 0)) return NULL; err = re_node_set_init_copy (&newstate->nodes, nodes); if (BE (err != REG_NOERROR, 0)) { re_free (newstate); return NULL; } newstate->entrance_nodes = &newstate->nodes; for (i = 0 ; i < nodes->nelem ; i++) { re_token_t *node = dfa->nodes + nodes->elems[i]; re_token_type_t type = node->type; if (type == CHARACTER && !node->constraint) continue; #ifdef RE_ENABLE_I18N newstate->accept_mb |= node->accept_mb; #endif /* RE_ENABLE_I18N */ /* If the state has the halt node, the state is a halt state. */ if (type == END_OF_RE) newstate->halt = 1; else if (type == OP_BACK_REF) newstate->has_backref = 1; else if (type == ANCHOR || node->constraint) newstate->has_constraint = 1; } err = register_state (dfa, newstate, hash); if (BE (err != REG_NOERROR, 0)) { free_state (newstate); newstate = NULL; } return newstate; } /* Create the new state which is depend on the context CONTEXT. Return the new state if succeeded, otherwise return NULL. */ static re_dfastate_t * internal_function __attribute_warn_unused_result__ create_cd_newstate (const re_dfa_t *dfa, const re_node_set *nodes, unsigned int context, re_hashval_t hash) { Idx i, nctx_nodes = 0; reg_errcode_t err; re_dfastate_t *newstate; newstate = (re_dfastate_t *) calloc (sizeof (re_dfastate_t), 1); if (BE (newstate == NULL, 0)) return NULL; err = re_node_set_init_copy (&newstate->nodes, nodes); if (BE (err != REG_NOERROR, 0)) { re_free (newstate); return NULL; } newstate->context = context; newstate->entrance_nodes = &newstate->nodes; for (i = 0 ; i < nodes->nelem ; i++) { re_token_t *node = dfa->nodes + nodes->elems[i]; re_token_type_t type = node->type; unsigned int constraint = node->constraint; if (type == CHARACTER && !constraint) continue; #ifdef RE_ENABLE_I18N newstate->accept_mb |= node->accept_mb; #endif /* RE_ENABLE_I18N */ /* If the state has the halt node, the state is a halt state. */ if (type == END_OF_RE) newstate->halt = 1; else if (type == OP_BACK_REF) newstate->has_backref = 1; if (constraint) { if (newstate->entrance_nodes == &newstate->nodes) { newstate->entrance_nodes = re_malloc (re_node_set, 1); if (BE (newstate->entrance_nodes == NULL, 0)) { free_state (newstate); return NULL; } if (re_node_set_init_copy (newstate->entrance_nodes, nodes) != REG_NOERROR) return NULL; nctx_nodes = 0; newstate->has_constraint = 1; } if (NOT_SATISFY_PREV_CONSTRAINT (constraint,context)) { re_node_set_remove_at (&newstate->nodes, i - nctx_nodes); ++nctx_nodes; } } } err = register_state (dfa, newstate, hash); if (BE (err != REG_NOERROR, 0)) { free_state (newstate); newstate = NULL; } return newstate; } gnuastro-0.2.33-8a3b/bootstrapped/lib/regex.c0000644000175000017500000000615313004436754015662 00000000000000/* Extended regular expression matching and search library. Copyright (C) 2002-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Contributed by Isamu Hasegawa . The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ #ifndef _LIBC # include # if (__GNUC__ == 4 && 6 <= __GNUC_MINOR__) || 4 < __GNUC__ # pragma GCC diagnostic ignored "-Wsuggest-attribute=pure" # endif # if (__GNUC__ == 4 && 3 <= __GNUC_MINOR__) || 4 < __GNUC__ # pragma GCC diagnostic ignored "-Wold-style-definition" # pragma GCC diagnostic ignored "-Wtype-limits" # endif #endif /* Make sure no one compiles this code with a C++ compiler. */ #if defined __cplusplus && defined _LIBC # error "This is C code, use a C compiler" #endif #ifdef _LIBC /* We have to keep the namespace clean. */ # define regfree(preg) __regfree (preg) # define regexec(pr, st, nm, pm, ef) __regexec (pr, st, nm, pm, ef) # define regcomp(preg, pattern, cflags) __regcomp (preg, pattern, cflags) # define regerror(errcode, preg, errbuf, errbuf_size) \ __regerror(errcode, preg, errbuf, errbuf_size) # define re_set_registers(bu, re, nu, st, en) \ __re_set_registers (bu, re, nu, st, en) # define re_match_2(bufp, string1, size1, string2, size2, pos, regs, stop) \ __re_match_2 (bufp, string1, size1, string2, size2, pos, regs, stop) # define re_match(bufp, string, size, pos, regs) \ __re_match (bufp, string, size, pos, regs) # define re_search(bufp, string, size, startpos, range, regs) \ __re_search (bufp, string, size, startpos, range, regs) # define re_compile_pattern(pattern, length, bufp) \ __re_compile_pattern (pattern, length, bufp) # define re_set_syntax(syntax) __re_set_syntax (syntax) # define re_search_2(bufp, st1, s1, st2, s2, startpos, range, regs, stop) \ __re_search_2 (bufp, st1, s1, st2, s2, startpos, range, regs, stop) # define re_compile_fastmap(bufp) __re_compile_fastmap (bufp) # include "../locale/localeinfo.h" #endif /* On some systems, limits.h sets RE_DUP_MAX to a lower value than GNU regex allows. Include it before , which correctly #undefs RE_DUP_MAX and sets it to the right value. */ #include #include #include "regex_internal.h" #include "regex_internal.c" #include "regcomp.c" #include "regexec.c" /* Binary backward compatibility. */ #if _LIBC # include # if SHLIB_COMPAT (libc, GLIBC_2_0, GLIBC_2_3) link_warning (re_max_failures, "the 're_max_failures' variable is obsolete and will go away.") int re_max_failures = 2000; # endif #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/regcomp.c0000644000175000017500000033544213004436754016212 00000000000000/* Extended regular expression matching and search library. Copyright (C) 2002-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Contributed by Isamu Hasegawa . The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ #ifdef _LIBC # include #endif static reg_errcode_t re_compile_internal (regex_t *preg, const char * pattern, size_t length, reg_syntax_t syntax); static void re_compile_fastmap_iter (regex_t *bufp, const re_dfastate_t *init_state, char *fastmap); static reg_errcode_t init_dfa (re_dfa_t *dfa, size_t pat_len); #ifdef RE_ENABLE_I18N static void free_charset (re_charset_t *cset); #endif /* RE_ENABLE_I18N */ static void free_workarea_compile (regex_t *preg); static reg_errcode_t create_initial_state (re_dfa_t *dfa); #ifdef RE_ENABLE_I18N static void optimize_utf8 (re_dfa_t *dfa); #endif static reg_errcode_t analyze (regex_t *preg); static reg_errcode_t preorder (bin_tree_t *root, reg_errcode_t (fn (void *, bin_tree_t *)), void *extra); static reg_errcode_t postorder (bin_tree_t *root, reg_errcode_t (fn (void *, bin_tree_t *)), void *extra); static reg_errcode_t optimize_subexps (void *extra, bin_tree_t *node); static reg_errcode_t lower_subexps (void *extra, bin_tree_t *node); static bin_tree_t *lower_subexp (reg_errcode_t *err, regex_t *preg, bin_tree_t *node); static reg_errcode_t calc_first (void *extra, bin_tree_t *node); static reg_errcode_t calc_next (void *extra, bin_tree_t *node); static reg_errcode_t link_nfa_nodes (void *extra, bin_tree_t *node); static Idx duplicate_node (re_dfa_t *dfa, Idx org_idx, unsigned int constraint); static Idx search_duplicated_node (const re_dfa_t *dfa, Idx org_node, unsigned int constraint); static reg_errcode_t calc_eclosure (re_dfa_t *dfa); static reg_errcode_t calc_eclosure_iter (re_node_set *new_set, re_dfa_t *dfa, Idx node, bool root); static reg_errcode_t calc_inveclosure (re_dfa_t *dfa); static Idx fetch_number (re_string_t *input, re_token_t *token, reg_syntax_t syntax); static int peek_token (re_token_t *token, re_string_t *input, reg_syntax_t syntax) internal_function; static bin_tree_t *parse (re_string_t *regexp, regex_t *preg, reg_syntax_t syntax, reg_errcode_t *err); static bin_tree_t *parse_reg_exp (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err); static bin_tree_t *parse_branch (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err); static bin_tree_t *parse_expression (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err); static bin_tree_t *parse_sub_exp (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err); static bin_tree_t *parse_dup_op (bin_tree_t *dup_elem, re_string_t *regexp, re_dfa_t *dfa, re_token_t *token, reg_syntax_t syntax, reg_errcode_t *err); static bin_tree_t *parse_bracket_exp (re_string_t *regexp, re_dfa_t *dfa, re_token_t *token, reg_syntax_t syntax, reg_errcode_t *err); static reg_errcode_t parse_bracket_element (bracket_elem_t *elem, re_string_t *regexp, re_token_t *token, int token_len, re_dfa_t *dfa, reg_syntax_t syntax, bool accept_hyphen); static reg_errcode_t parse_bracket_symbol (bracket_elem_t *elem, re_string_t *regexp, re_token_t *token); #ifdef RE_ENABLE_I18N static reg_errcode_t build_equiv_class (bitset_t sbcset, re_charset_t *mbcset, Idx *equiv_class_alloc, const unsigned char *name); static reg_errcode_t build_charclass (RE_TRANSLATE_TYPE trans, bitset_t sbcset, re_charset_t *mbcset, Idx *char_class_alloc, const char *class_name, reg_syntax_t syntax); #else /* not RE_ENABLE_I18N */ static reg_errcode_t build_equiv_class (bitset_t sbcset, const unsigned char *name); static reg_errcode_t build_charclass (RE_TRANSLATE_TYPE trans, bitset_t sbcset, const char *class_name, reg_syntax_t syntax); #endif /* not RE_ENABLE_I18N */ static bin_tree_t *build_charclass_op (re_dfa_t *dfa, RE_TRANSLATE_TYPE trans, const char *class_name, const char *extra, bool non_match, reg_errcode_t *err); static bin_tree_t *create_tree (re_dfa_t *dfa, bin_tree_t *left, bin_tree_t *right, re_token_type_t type); static bin_tree_t *create_token_tree (re_dfa_t *dfa, bin_tree_t *left, bin_tree_t *right, const re_token_t *token); static bin_tree_t *duplicate_tree (const bin_tree_t *src, re_dfa_t *dfa); static void free_token (re_token_t *node); static reg_errcode_t free_tree (void *extra, bin_tree_t *node); static reg_errcode_t mark_opt_subexp (void *extra, bin_tree_t *node); /* This table gives an error message for each of the error codes listed in regex.h. Obviously the order here has to be same as there. POSIX doesn't require that we do anything for REG_NOERROR, but why not be nice? */ static const char __re_error_msgid[] = { #define REG_NOERROR_IDX 0 gettext_noop ("Success") /* REG_NOERROR */ "\0" #define REG_NOMATCH_IDX (REG_NOERROR_IDX + sizeof "Success") gettext_noop ("No match") /* REG_NOMATCH */ "\0" #define REG_BADPAT_IDX (REG_NOMATCH_IDX + sizeof "No match") gettext_noop ("Invalid regular expression") /* REG_BADPAT */ "\0" #define REG_ECOLLATE_IDX (REG_BADPAT_IDX + sizeof "Invalid regular expression") gettext_noop ("Invalid collation character") /* REG_ECOLLATE */ "\0" #define REG_ECTYPE_IDX (REG_ECOLLATE_IDX + sizeof "Invalid collation character") gettext_noop ("Invalid character class name") /* REG_ECTYPE */ "\0" #define REG_EESCAPE_IDX (REG_ECTYPE_IDX + sizeof "Invalid character class name") gettext_noop ("Trailing backslash") /* REG_EESCAPE */ "\0" #define REG_ESUBREG_IDX (REG_EESCAPE_IDX + sizeof "Trailing backslash") gettext_noop ("Invalid back reference") /* REG_ESUBREG */ "\0" #define REG_EBRACK_IDX (REG_ESUBREG_IDX + sizeof "Invalid back reference") gettext_noop ("Unmatched [, [^, [:, [., or [=") /* REG_EBRACK */ "\0" #define REG_EPAREN_IDX (REG_EBRACK_IDX + sizeof "Unmatched [, [^, [:, [., or [=") gettext_noop ("Unmatched ( or \\(") /* REG_EPAREN */ "\0" #define REG_EBRACE_IDX (REG_EPAREN_IDX + sizeof "Unmatched ( or \\(") gettext_noop ("Unmatched \\{") /* REG_EBRACE */ "\0" #define REG_BADBR_IDX (REG_EBRACE_IDX + sizeof "Unmatched \\{") gettext_noop ("Invalid content of \\{\\}") /* REG_BADBR */ "\0" #define REG_ERANGE_IDX (REG_BADBR_IDX + sizeof "Invalid content of \\{\\}") gettext_noop ("Invalid range end") /* REG_ERANGE */ "\0" #define REG_ESPACE_IDX (REG_ERANGE_IDX + sizeof "Invalid range end") gettext_noop ("Memory exhausted") /* REG_ESPACE */ "\0" #define REG_BADRPT_IDX (REG_ESPACE_IDX + sizeof "Memory exhausted") gettext_noop ("Invalid preceding regular expression") /* REG_BADRPT */ "\0" #define REG_EEND_IDX (REG_BADRPT_IDX + sizeof "Invalid preceding regular expression") gettext_noop ("Premature end of regular expression") /* REG_EEND */ "\0" #define REG_ESIZE_IDX (REG_EEND_IDX + sizeof "Premature end of regular expression") gettext_noop ("Regular expression too big") /* REG_ESIZE */ "\0" #define REG_ERPAREN_IDX (REG_ESIZE_IDX + sizeof "Regular expression too big") gettext_noop ("Unmatched ) or \\)") /* REG_ERPAREN */ }; static const size_t __re_error_msgid_idx[] = { REG_NOERROR_IDX, REG_NOMATCH_IDX, REG_BADPAT_IDX, REG_ECOLLATE_IDX, REG_ECTYPE_IDX, REG_EESCAPE_IDX, REG_ESUBREG_IDX, REG_EBRACK_IDX, REG_EPAREN_IDX, REG_EBRACE_IDX, REG_BADBR_IDX, REG_ERANGE_IDX, REG_ESPACE_IDX, REG_BADRPT_IDX, REG_EEND_IDX, REG_ESIZE_IDX, REG_ERPAREN_IDX }; /* Entry points for GNU code. */ /* re_compile_pattern is the GNU regular expression compiler: it compiles PATTERN (of length LENGTH) and puts the result in BUFP. Returns 0 if the pattern was valid, otherwise an error string. Assumes the 'allocated' (and perhaps 'buffer') and 'translate' fields are set in BUFP on entry. */ const char * re_compile_pattern (const char *pattern, size_t length, struct re_pattern_buffer *bufp) { reg_errcode_t ret; /* And GNU code determines whether or not to get register information by passing null for the REGS argument to re_match, etc., not by setting no_sub, unless RE_NO_SUB is set. */ bufp->no_sub = !!(re_syntax_options & RE_NO_SUB); /* Match anchors at newline. */ bufp->newline_anchor = 1; ret = re_compile_internal (bufp, pattern, length, re_syntax_options); if (!ret) return NULL; return gettext (__re_error_msgid + __re_error_msgid_idx[(int) ret]); } #ifdef _LIBC weak_alias (__re_compile_pattern, re_compile_pattern) #endif /* Set by 're_set_syntax' to the current regexp syntax to recognize. Can also be assigned to arbitrarily: each pattern buffer stores its own syntax, so it can be changed between regex compilations. */ /* This has no initializer because initialized variables in Emacs become read-only after dumping. */ reg_syntax_t re_syntax_options; /* Specify the precise syntax of regexps for compilation. This provides for compatibility for various utilities which historically have different, incompatible syntaxes. The argument SYNTAX is a bit mask comprised of the various bits defined in regex.h. We return the old syntax. */ reg_syntax_t re_set_syntax (reg_syntax_t syntax) { reg_syntax_t ret = re_syntax_options; re_syntax_options = syntax; return ret; } #ifdef _LIBC weak_alias (__re_set_syntax, re_set_syntax) #endif int re_compile_fastmap (struct re_pattern_buffer *bufp) { re_dfa_t *dfa = bufp->buffer; char *fastmap = bufp->fastmap; memset (fastmap, '\0', sizeof (char) * SBC_MAX); re_compile_fastmap_iter (bufp, dfa->init_state, fastmap); if (dfa->init_state != dfa->init_state_word) re_compile_fastmap_iter (bufp, dfa->init_state_word, fastmap); if (dfa->init_state != dfa->init_state_nl) re_compile_fastmap_iter (bufp, dfa->init_state_nl, fastmap); if (dfa->init_state != dfa->init_state_begbuf) re_compile_fastmap_iter (bufp, dfa->init_state_begbuf, fastmap); bufp->fastmap_accurate = 1; return 0; } #ifdef _LIBC weak_alias (__re_compile_fastmap, re_compile_fastmap) #endif static inline void __attribute__ ((always_inline)) re_set_fastmap (char *fastmap, bool icase, int ch) { fastmap[ch] = 1; if (icase) fastmap[tolower (ch)] = 1; } /* Helper function for re_compile_fastmap. Compile fastmap for the initial_state INIT_STATE. */ static void re_compile_fastmap_iter (regex_t *bufp, const re_dfastate_t *init_state, char *fastmap) { re_dfa_t *dfa = bufp->buffer; Idx node_cnt; bool icase = (dfa->mb_cur_max == 1 && (bufp->syntax & RE_ICASE)); for (node_cnt = 0; node_cnt < init_state->nodes.nelem; ++node_cnt) { Idx node = init_state->nodes.elems[node_cnt]; re_token_type_t type = dfa->nodes[node].type; if (type == CHARACTER) { re_set_fastmap (fastmap, icase, dfa->nodes[node].opr.c); #ifdef RE_ENABLE_I18N if ((bufp->syntax & RE_ICASE) && dfa->mb_cur_max > 1) { unsigned char buf[MB_LEN_MAX]; unsigned char *p; wchar_t wc; mbstate_t state; p = buf; *p++ = dfa->nodes[node].opr.c; while (++node < dfa->nodes_len && dfa->nodes[node].type == CHARACTER && dfa->nodes[node].mb_partial) *p++ = dfa->nodes[node].opr.c; memset (&state, '\0', sizeof (state)); if (__mbrtowc (&wc, (const char *) buf, p - buf, &state) == p - buf && (__wcrtomb ((char *) buf, __towlower (wc), &state) != (size_t) -1)) re_set_fastmap (fastmap, false, buf[0]); } #endif } else if (type == SIMPLE_BRACKET) { int i, ch; for (i = 0, ch = 0; i < BITSET_WORDS; ++i) { int j; bitset_word_t w = dfa->nodes[node].opr.sbcset[i]; for (j = 0; j < BITSET_WORD_BITS; ++j, ++ch) if (w & ((bitset_word_t) 1 << j)) re_set_fastmap (fastmap, icase, ch); } } #ifdef RE_ENABLE_I18N else if (type == COMPLEX_BRACKET) { re_charset_t *cset = dfa->nodes[node].opr.mbcset; Idx i; # ifdef _LIBC /* See if we have to try all bytes which start multiple collation elements. e.g. In da_DK, we want to catch 'a' since "aa" is a valid collation element, and don't catch 'b' since 'b' is the only collation element which starts from 'b' (and it is caught by SIMPLE_BRACKET). */ if (_NL_CURRENT_WORD (LC_COLLATE, _NL_COLLATE_NRULES) != 0 && (cset->ncoll_syms || cset->nranges)) { const int32_t *table = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_TABLEMB); for (i = 0; i < SBC_MAX; ++i) if (table[i] < 0) re_set_fastmap (fastmap, icase, i); } # endif /* _LIBC */ /* See if we have to start the match at all multibyte characters, i.e. where we would not find an invalid sequence. This only applies to multibyte character sets; for single byte character sets, the SIMPLE_BRACKET again suffices. */ if (dfa->mb_cur_max > 1 && (cset->nchar_classes || cset->non_match || cset->nranges # ifdef _LIBC || cset->nequiv_classes # endif /* _LIBC */ )) { unsigned char c = 0; do { mbstate_t mbs; memset (&mbs, 0, sizeof (mbs)); if (__mbrtowc (NULL, (char *) &c, 1, &mbs) == (size_t) -2) re_set_fastmap (fastmap, false, (int) c); } while (++c != 0); } else { /* ... Else catch all bytes which can start the mbchars. */ for (i = 0; i < cset->nmbchars; ++i) { char buf[256]; mbstate_t state; memset (&state, '\0', sizeof (state)); if (__wcrtomb (buf, cset->mbchars[i], &state) != (size_t) -1) re_set_fastmap (fastmap, icase, *(unsigned char *) buf); if ((bufp->syntax & RE_ICASE) && dfa->mb_cur_max > 1) { if (__wcrtomb (buf, __towlower (cset->mbchars[i]), &state) != (size_t) -1) re_set_fastmap (fastmap, false, *(unsigned char *) buf); } } } } #endif /* RE_ENABLE_I18N */ else if (type == OP_PERIOD #ifdef RE_ENABLE_I18N || type == OP_UTF8_PERIOD #endif /* RE_ENABLE_I18N */ || type == END_OF_RE) { memset (fastmap, '\1', sizeof (char) * SBC_MAX); if (type == END_OF_RE) bufp->can_be_null = 1; return; } } } /* Entry point for POSIX code. */ /* regcomp takes a regular expression as a string and compiles it. PREG is a regex_t *. We do not expect any fields to be initialized, since POSIX says we shouldn't. Thus, we set 'buffer' to the compiled pattern; 'used' to the length of the compiled pattern; 'syntax' to RE_SYNTAX_POSIX_EXTENDED if the REG_EXTENDED bit in CFLAGS is set; otherwise, to RE_SYNTAX_POSIX_BASIC; 'newline_anchor' to REG_NEWLINE being set in CFLAGS; 'fastmap' to an allocated space for the fastmap; 'fastmap_accurate' to zero; 're_nsub' to the number of subexpressions in PATTERN. PATTERN is the address of the pattern string. CFLAGS is a series of bits which affect compilation. If REG_EXTENDED is set, we use POSIX extended syntax; otherwise, we use POSIX basic syntax. If REG_NEWLINE is set, then . and [^...] don't match newline. Also, regexec will try a match beginning after every newline. If REG_ICASE is set, then we considers upper- and lowercase versions of letters to be equivalent when matching. If REG_NOSUB is set, then when PREG is passed to regexec, that routine will report only success or failure, and nothing about the registers. It returns 0 if it succeeds, nonzero if it doesn't. (See regex.h for the return codes and their meanings.) */ int regcomp (regex_t *_Restrict_ preg, const char *_Restrict_ pattern, int cflags) { reg_errcode_t ret; reg_syntax_t syntax = ((cflags & REG_EXTENDED) ? RE_SYNTAX_POSIX_EXTENDED : RE_SYNTAX_POSIX_BASIC); preg->buffer = NULL; preg->allocated = 0; preg->used = 0; /* Try to allocate space for the fastmap. */ preg->fastmap = re_malloc (char, SBC_MAX); if (BE (preg->fastmap == NULL, 0)) return REG_ESPACE; syntax |= (cflags & REG_ICASE) ? RE_ICASE : 0; /* If REG_NEWLINE is set, newlines are treated differently. */ if (cflags & REG_NEWLINE) { /* REG_NEWLINE implies neither . nor [^...] match newline. */ syntax &= ~RE_DOT_NEWLINE; syntax |= RE_HAT_LISTS_NOT_NEWLINE; /* It also changes the matching behavior. */ preg->newline_anchor = 1; } else preg->newline_anchor = 0; preg->no_sub = !!(cflags & REG_NOSUB); preg->translate = NULL; ret = re_compile_internal (preg, pattern, strlen (pattern), syntax); /* POSIX doesn't distinguish between an unmatched open-group and an unmatched close-group: both are REG_EPAREN. */ if (ret == REG_ERPAREN) ret = REG_EPAREN; /* We have already checked preg->fastmap != NULL. */ if (BE (ret == REG_NOERROR, 1)) /* Compute the fastmap now, since regexec cannot modify the pattern buffer. This function never fails in this implementation. */ (void) re_compile_fastmap (preg); else { /* Some error occurred while compiling the expression. */ re_free (preg->fastmap); preg->fastmap = NULL; } return (int) ret; } #ifdef _LIBC weak_alias (__regcomp, regcomp) #endif /* Returns a message corresponding to an error code, ERRCODE, returned from either regcomp or regexec. We don't use PREG here. */ size_t regerror (int errcode, const regex_t *_Restrict_ preg, char *_Restrict_ errbuf, size_t errbuf_size) { const char *msg; size_t msg_size; if (BE (errcode < 0 || errcode >= (int) (sizeof (__re_error_msgid_idx) / sizeof (__re_error_msgid_idx[0])), 0)) /* Only error codes returned by the rest of the code should be passed to this routine. If we are given anything else, or if other regex code generates an invalid error code, then the program has a bug. Dump core so we can fix it. */ abort (); msg = gettext (__re_error_msgid + __re_error_msgid_idx[errcode]); msg_size = strlen (msg) + 1; /* Includes the null. */ if (BE (errbuf_size != 0, 1)) { size_t cpy_size = msg_size; if (BE (msg_size > errbuf_size, 0)) { cpy_size = errbuf_size - 1; errbuf[cpy_size] = '\0'; } memcpy (errbuf, msg, cpy_size); } return msg_size; } #ifdef _LIBC weak_alias (__regerror, regerror) #endif #ifdef RE_ENABLE_I18N /* This static array is used for the map to single-byte characters when UTF-8 is used. Otherwise we would allocate memory just to initialize it the same all the time. UTF-8 is the preferred encoding so this is a worthwhile optimization. */ static const bitset_t utf8_sb_map = { /* Set the first 128 bits. */ # if defined __GNUC__ && !defined __STRICT_ANSI__ [0 ... 0x80 / BITSET_WORD_BITS - 1] = BITSET_WORD_MAX # else # if 4 * BITSET_WORD_BITS < ASCII_CHARS # error "bitset_word_t is narrower than 32 bits" # elif 3 * BITSET_WORD_BITS < ASCII_CHARS BITSET_WORD_MAX, BITSET_WORD_MAX, BITSET_WORD_MAX, # elif 2 * BITSET_WORD_BITS < ASCII_CHARS BITSET_WORD_MAX, BITSET_WORD_MAX, # elif 1 * BITSET_WORD_BITS < ASCII_CHARS BITSET_WORD_MAX, # endif (BITSET_WORD_MAX >> (SBC_MAX % BITSET_WORD_BITS == 0 ? 0 : BITSET_WORD_BITS - SBC_MAX % BITSET_WORD_BITS)) # endif }; #endif static void free_dfa_content (re_dfa_t *dfa) { Idx i, j; if (dfa->nodes) for (i = 0; i < dfa->nodes_len; ++i) free_token (dfa->nodes + i); re_free (dfa->nexts); for (i = 0; i < dfa->nodes_len; ++i) { if (dfa->eclosures != NULL) re_node_set_free (dfa->eclosures + i); if (dfa->inveclosures != NULL) re_node_set_free (dfa->inveclosures + i); if (dfa->edests != NULL) re_node_set_free (dfa->edests + i); } re_free (dfa->edests); re_free (dfa->eclosures); re_free (dfa->inveclosures); re_free (dfa->nodes); if (dfa->state_table) for (i = 0; i <= dfa->state_hash_mask; ++i) { struct re_state_table_entry *entry = dfa->state_table + i; for (j = 0; j < entry->num; ++j) { re_dfastate_t *state = entry->array[j]; free_state (state); } re_free (entry->array); } re_free (dfa->state_table); #ifdef RE_ENABLE_I18N if (dfa->sb_char != utf8_sb_map) re_free (dfa->sb_char); #endif re_free (dfa->subexp_map); #ifdef DEBUG re_free (dfa->re_str); #endif re_free (dfa); } /* Free dynamically allocated space used by PREG. */ void regfree (regex_t *preg) { re_dfa_t *dfa = preg->buffer; if (BE (dfa != NULL, 1)) { lock_fini (dfa->lock); free_dfa_content (dfa); } preg->buffer = NULL; preg->allocated = 0; re_free (preg->fastmap); preg->fastmap = NULL; re_free (preg->translate); preg->translate = NULL; } #ifdef _LIBC weak_alias (__regfree, regfree) #endif /* Entry points compatible with 4.2 BSD regex library. We don't define them unless specifically requested. */ #if defined _REGEX_RE_COMP || defined _LIBC /* BSD has one and only one pattern buffer. */ static struct re_pattern_buffer re_comp_buf; char * # ifdef _LIBC /* Make these definitions weak in libc, so POSIX programs can redefine these names if they don't use our functions, and still use regcomp/regexec above without link errors. */ weak_function # endif re_comp (const char *s) { reg_errcode_t ret; char *fastmap; if (!s) { if (!re_comp_buf.buffer) return gettext ("No previous regular expression"); return 0; } if (re_comp_buf.buffer) { fastmap = re_comp_buf.fastmap; re_comp_buf.fastmap = NULL; __regfree (&re_comp_buf); memset (&re_comp_buf, '\0', sizeof (re_comp_buf)); re_comp_buf.fastmap = fastmap; } if (re_comp_buf.fastmap == NULL) { re_comp_buf.fastmap = (char *) malloc (SBC_MAX); if (re_comp_buf.fastmap == NULL) return (char *) gettext (__re_error_msgid + __re_error_msgid_idx[(int) REG_ESPACE]); } /* Since 're_exec' always passes NULL for the 'regs' argument, we don't need to initialize the pattern buffer fields which affect it. */ /* Match anchors at newlines. */ re_comp_buf.newline_anchor = 1; ret = re_compile_internal (&re_comp_buf, s, strlen (s), re_syntax_options); if (!ret) return NULL; /* Yes, we're discarding 'const' here if !HAVE_LIBINTL. */ return (char *) gettext (__re_error_msgid + __re_error_msgid_idx[(int) ret]); } #ifdef _LIBC libc_freeres_fn (free_mem) { __regfree (&re_comp_buf); } #endif #endif /* _REGEX_RE_COMP */ /* Internal entry point. Compile the regular expression PATTERN, whose length is LENGTH. SYNTAX indicate regular expression's syntax. */ static reg_errcode_t re_compile_internal (regex_t *preg, const char * pattern, size_t length, reg_syntax_t syntax) { reg_errcode_t err = REG_NOERROR; re_dfa_t *dfa; re_string_t regexp; /* Initialize the pattern buffer. */ preg->fastmap_accurate = 0; preg->syntax = syntax; preg->not_bol = preg->not_eol = 0; preg->used = 0; preg->re_nsub = 0; preg->can_be_null = 0; preg->regs_allocated = REGS_UNALLOCATED; /* Initialize the dfa. */ dfa = preg->buffer; if (BE (preg->allocated < sizeof (re_dfa_t), 0)) { /* If zero allocated, but buffer is non-null, try to realloc enough space. This loses if buffer's address is bogus, but that is the user's responsibility. If ->buffer is NULL this is a simple allocation. */ dfa = re_realloc (preg->buffer, re_dfa_t, 1); if (dfa == NULL) return REG_ESPACE; preg->allocated = sizeof (re_dfa_t); preg->buffer = dfa; } preg->used = sizeof (re_dfa_t); err = init_dfa (dfa, length); if (BE (err == REG_NOERROR && lock_init (dfa->lock) != 0, 0)) err = REG_ESPACE; if (BE (err != REG_NOERROR, 0)) { free_dfa_content (dfa); preg->buffer = NULL; preg->allocated = 0; return err; } #ifdef DEBUG /* Note: length+1 will not overflow since it is checked in init_dfa. */ dfa->re_str = re_malloc (char, length + 1); strncpy (dfa->re_str, pattern, length + 1); #endif err = re_string_construct (®exp, pattern, length, preg->translate, (syntax & RE_ICASE) != 0, dfa); if (BE (err != REG_NOERROR, 0)) { re_compile_internal_free_return: free_workarea_compile (preg); re_string_destruct (®exp); lock_fini (dfa->lock); free_dfa_content (dfa); preg->buffer = NULL; preg->allocated = 0; return err; } /* Parse the regular expression, and build a structure tree. */ preg->re_nsub = 0; dfa->str_tree = parse (®exp, preg, syntax, &err); if (BE (dfa->str_tree == NULL, 0)) goto re_compile_internal_free_return; /* Analyze the tree and create the nfa. */ err = analyze (preg); if (BE (err != REG_NOERROR, 0)) goto re_compile_internal_free_return; #ifdef RE_ENABLE_I18N /* If possible, do searching in single byte encoding to speed things up. */ if (dfa->is_utf8 && !(syntax & RE_ICASE) && preg->translate == NULL) optimize_utf8 (dfa); #endif /* Then create the initial state of the dfa. */ err = create_initial_state (dfa); /* Release work areas. */ free_workarea_compile (preg); re_string_destruct (®exp); if (BE (err != REG_NOERROR, 0)) { lock_fini (dfa->lock); free_dfa_content (dfa); preg->buffer = NULL; preg->allocated = 0; } return err; } /* Initialize DFA. We use the length of the regular expression PAT_LEN as the initial length of some arrays. */ static reg_errcode_t init_dfa (re_dfa_t *dfa, size_t pat_len) { __re_size_t table_size; #ifndef _LIBC const char *codeset_name; #endif #ifdef RE_ENABLE_I18N size_t max_i18n_object_size = MAX (sizeof (wchar_t), sizeof (wctype_t)); #else size_t max_i18n_object_size = 0; #endif size_t max_object_size = MAX (sizeof (struct re_state_table_entry), MAX (sizeof (re_token_t), MAX (sizeof (re_node_set), MAX (sizeof (regmatch_t), max_i18n_object_size)))); memset (dfa, '\0', sizeof (re_dfa_t)); /* Force allocation of str_tree_storage the first time. */ dfa->str_tree_storage_idx = BIN_TREE_STORAGE_SIZE; /* Avoid overflows. The extra "/ 2" is for the table_size doubling calculation below, and for similar doubling calculations elsewhere. And it's <= rather than <, because some of the doubling calculations add 1 afterwards. */ if (BE (MIN (IDX_MAX, SIZE_MAX / max_object_size) / 2 <= pat_len, 0)) return REG_ESPACE; dfa->nodes_alloc = pat_len + 1; dfa->nodes = re_malloc (re_token_t, dfa->nodes_alloc); /* table_size = 2 ^ ceil(log pat_len) */ for (table_size = 1; ; table_size <<= 1) if (table_size > pat_len) break; dfa->state_table = calloc (sizeof (struct re_state_table_entry), table_size); dfa->state_hash_mask = table_size - 1; dfa->mb_cur_max = MB_CUR_MAX; #ifdef _LIBC if (dfa->mb_cur_max == 6 && strcmp (_NL_CURRENT (LC_CTYPE, _NL_CTYPE_CODESET_NAME), "UTF-8") == 0) dfa->is_utf8 = 1; dfa->map_notascii = (_NL_CURRENT_WORD (LC_CTYPE, _NL_CTYPE_MAP_TO_NONASCII) != 0); #else codeset_name = nl_langinfo (CODESET); if ((codeset_name[0] == 'U' || codeset_name[0] == 'u') && (codeset_name[1] == 'T' || codeset_name[1] == 't') && (codeset_name[2] == 'F' || codeset_name[2] == 'f') && strcmp (codeset_name + 3 + (codeset_name[3] == '-'), "8") == 0) dfa->is_utf8 = 1; /* We check exhaustively in the loop below if this charset is a superset of ASCII. */ dfa->map_notascii = 0; #endif #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) { if (dfa->is_utf8) dfa->sb_char = (re_bitset_ptr_t) utf8_sb_map; else { int i, j, ch; dfa->sb_char = (re_bitset_ptr_t) calloc (sizeof (bitset_t), 1); if (BE (dfa->sb_char == NULL, 0)) return REG_ESPACE; /* Set the bits corresponding to single byte chars. */ for (i = 0, ch = 0; i < BITSET_WORDS; ++i) for (j = 0; j < BITSET_WORD_BITS; ++j, ++ch) { wint_t wch = __btowc (ch); if (wch != WEOF) dfa->sb_char[i] |= (bitset_word_t) 1 << j; # ifndef _LIBC if (isascii (ch) && wch != ch) dfa->map_notascii = 1; # endif } } } #endif if (BE (dfa->nodes == NULL || dfa->state_table == NULL, 0)) return REG_ESPACE; return REG_NOERROR; } /* Initialize WORD_CHAR table, which indicate which character is "word". In this case "word" means that it is the word construction character used by some operators like "\<", "\>", etc. */ static void internal_function init_word_char (re_dfa_t *dfa) { int i = 0; int j; int ch = 0; dfa->word_ops_used = 1; if (BE (dfa->map_notascii == 0, 1)) { bitset_word_t bits0 = 0x00000000; bitset_word_t bits1 = 0x03ff0000; bitset_word_t bits2 = 0x87fffffe; bitset_word_t bits3 = 0x07fffffe; if (BITSET_WORD_BITS == 64) { dfa->word_char[0] = bits1 << 31 << 1 | bits0; dfa->word_char[1] = bits3 << 31 << 1 | bits2; i = 2; } else if (BITSET_WORD_BITS == 32) { dfa->word_char[0] = bits0; dfa->word_char[1] = bits1; dfa->word_char[2] = bits2; dfa->word_char[3] = bits3; i = 4; } else goto general_case; ch = 128; if (BE (dfa->is_utf8, 1)) { memset (&dfa->word_char[i], '\0', (SBC_MAX - ch) / 8); return; } } general_case: for (; i < BITSET_WORDS; ++i) for (j = 0; j < BITSET_WORD_BITS; ++j, ++ch) if (isalnum (ch) || ch == '_') dfa->word_char[i] |= (bitset_word_t) 1 << j; } /* Free the work area which are only used while compiling. */ static void free_workarea_compile (regex_t *preg) { re_dfa_t *dfa = preg->buffer; bin_tree_storage_t *storage, *next; for (storage = dfa->str_tree_storage; storage; storage = next) { next = storage->next; re_free (storage); } dfa->str_tree_storage = NULL; dfa->str_tree_storage_idx = BIN_TREE_STORAGE_SIZE; dfa->str_tree = NULL; re_free (dfa->org_indices); dfa->org_indices = NULL; } /* Create initial states for all contexts. */ static reg_errcode_t create_initial_state (re_dfa_t *dfa) { Idx first, i; reg_errcode_t err; re_node_set init_nodes; /* Initial states have the epsilon closure of the node which is the first node of the regular expression. */ first = dfa->str_tree->first->node_idx; dfa->init_node = first; err = re_node_set_init_copy (&init_nodes, dfa->eclosures + first); if (BE (err != REG_NOERROR, 0)) return err; /* The back-references which are in initial states can epsilon transit, since in this case all of the subexpressions can be null. Then we add epsilon closures of the nodes which are the next nodes of the back-references. */ if (dfa->nbackref > 0) for (i = 0; i < init_nodes.nelem; ++i) { Idx node_idx = init_nodes.elems[i]; re_token_type_t type = dfa->nodes[node_idx].type; Idx clexp_idx; if (type != OP_BACK_REF) continue; for (clexp_idx = 0; clexp_idx < init_nodes.nelem; ++clexp_idx) { re_token_t *clexp_node; clexp_node = dfa->nodes + init_nodes.elems[clexp_idx]; if (clexp_node->type == OP_CLOSE_SUBEXP && clexp_node->opr.idx == dfa->nodes[node_idx].opr.idx) break; } if (clexp_idx == init_nodes.nelem) continue; if (type == OP_BACK_REF) { Idx dest_idx = dfa->edests[node_idx].elems[0]; if (!re_node_set_contains (&init_nodes, dest_idx)) { reg_errcode_t merge_err = re_node_set_merge (&init_nodes, dfa->eclosures + dest_idx); if (merge_err != REG_NOERROR) return merge_err; i = 0; } } } /* It must be the first time to invoke acquire_state. */ dfa->init_state = re_acquire_state_context (&err, dfa, &init_nodes, 0); /* We don't check ERR here, since the initial state must not be NULL. */ if (BE (dfa->init_state == NULL, 0)) return err; if (dfa->init_state->has_constraint) { dfa->init_state_word = re_acquire_state_context (&err, dfa, &init_nodes, CONTEXT_WORD); dfa->init_state_nl = re_acquire_state_context (&err, dfa, &init_nodes, CONTEXT_NEWLINE); dfa->init_state_begbuf = re_acquire_state_context (&err, dfa, &init_nodes, CONTEXT_NEWLINE | CONTEXT_BEGBUF); if (BE (dfa->init_state_word == NULL || dfa->init_state_nl == NULL || dfa->init_state_begbuf == NULL, 0)) return err; } else dfa->init_state_word = dfa->init_state_nl = dfa->init_state_begbuf = dfa->init_state; re_node_set_free (&init_nodes); return REG_NOERROR; } #ifdef RE_ENABLE_I18N /* If it is possible to do searching in single byte encoding instead of UTF-8 to speed things up, set dfa->mb_cur_max to 1, clear is_utf8 and change DFA nodes where needed. */ static void optimize_utf8 (re_dfa_t *dfa) { Idx node; int i; bool mb_chars = false; bool has_period = false; for (node = 0; node < dfa->nodes_len; ++node) switch (dfa->nodes[node].type) { case CHARACTER: if (dfa->nodes[node].opr.c >= ASCII_CHARS) mb_chars = true; break; case ANCHOR: switch (dfa->nodes[node].opr.ctx_type) { case LINE_FIRST: case LINE_LAST: case BUF_FIRST: case BUF_LAST: break; default: /* Word anchors etc. cannot be handled. It's okay to test opr.ctx_type since constraints (for all DFA nodes) are created by ORing one or more opr.ctx_type values. */ return; } break; case OP_PERIOD: has_period = true; break; case OP_BACK_REF: case OP_ALT: case END_OF_RE: case OP_DUP_ASTERISK: case OP_OPEN_SUBEXP: case OP_CLOSE_SUBEXP: break; case COMPLEX_BRACKET: return; case SIMPLE_BRACKET: /* Just double check. */ { int rshift = (ASCII_CHARS % BITSET_WORD_BITS == 0 ? 0 : BITSET_WORD_BITS - ASCII_CHARS % BITSET_WORD_BITS); for (i = ASCII_CHARS / BITSET_WORD_BITS; i < BITSET_WORDS; ++i) { if (dfa->nodes[node].opr.sbcset[i] >> rshift != 0) return; rshift = 0; } } break; default: abort (); } if (mb_chars || has_period) for (node = 0; node < dfa->nodes_len; ++node) { if (dfa->nodes[node].type == CHARACTER && dfa->nodes[node].opr.c >= ASCII_CHARS) dfa->nodes[node].mb_partial = 0; else if (dfa->nodes[node].type == OP_PERIOD) dfa->nodes[node].type = OP_UTF8_PERIOD; } /* The search can be in single byte locale. */ dfa->mb_cur_max = 1; dfa->is_utf8 = 0; dfa->has_mb_node = dfa->nbackref > 0 || has_period; } #endif /* Analyze the structure tree, and calculate "first", "next", "edest", "eclosure", and "inveclosure". */ static reg_errcode_t analyze (regex_t *preg) { re_dfa_t *dfa = preg->buffer; reg_errcode_t ret; /* Allocate arrays. */ dfa->nexts = re_malloc (Idx, dfa->nodes_alloc); dfa->org_indices = re_malloc (Idx, dfa->nodes_alloc); dfa->edests = re_malloc (re_node_set, dfa->nodes_alloc); dfa->eclosures = re_malloc (re_node_set, dfa->nodes_alloc); if (BE (dfa->nexts == NULL || dfa->org_indices == NULL || dfa->edests == NULL || dfa->eclosures == NULL, 0)) return REG_ESPACE; dfa->subexp_map = re_malloc (Idx, preg->re_nsub); if (dfa->subexp_map != NULL) { Idx i; for (i = 0; i < preg->re_nsub; i++) dfa->subexp_map[i] = i; preorder (dfa->str_tree, optimize_subexps, dfa); for (i = 0; i < preg->re_nsub; i++) if (dfa->subexp_map[i] != i) break; if (i == preg->re_nsub) { free (dfa->subexp_map); dfa->subexp_map = NULL; } } ret = postorder (dfa->str_tree, lower_subexps, preg); if (BE (ret != REG_NOERROR, 0)) return ret; ret = postorder (dfa->str_tree, calc_first, dfa); if (BE (ret != REG_NOERROR, 0)) return ret; preorder (dfa->str_tree, calc_next, dfa); ret = preorder (dfa->str_tree, link_nfa_nodes, dfa); if (BE (ret != REG_NOERROR, 0)) return ret; ret = calc_eclosure (dfa); if (BE (ret != REG_NOERROR, 0)) return ret; /* We only need this during the prune_impossible_nodes pass in regexec.c; skip it if p_i_n will not run, as calc_inveclosure can be quadratic. */ if ((!preg->no_sub && preg->re_nsub > 0 && dfa->has_plural_match) || dfa->nbackref) { dfa->inveclosures = re_malloc (re_node_set, dfa->nodes_len); if (BE (dfa->inveclosures == NULL, 0)) return REG_ESPACE; ret = calc_inveclosure (dfa); } return ret; } /* Our parse trees are very unbalanced, so we cannot use a stack to implement parse tree visits. Instead, we use parent pointers and some hairy code in these two functions. */ static reg_errcode_t postorder (bin_tree_t *root, reg_errcode_t (fn (void *, bin_tree_t *)), void *extra) { bin_tree_t *node, *prev; for (node = root; ; ) { /* Descend down the tree, preferably to the left (or to the right if that's the only child). */ while (node->left || node->right) if (node->left) node = node->left; else node = node->right; do { reg_errcode_t err = fn (extra, node); if (BE (err != REG_NOERROR, 0)) return err; if (node->parent == NULL) return REG_NOERROR; prev = node; node = node->parent; } /* Go up while we have a node that is reached from the right. */ while (node->right == prev || node->right == NULL); node = node->right; } } static reg_errcode_t preorder (bin_tree_t *root, reg_errcode_t (fn (void *, bin_tree_t *)), void *extra) { bin_tree_t *node; for (node = root; ; ) { reg_errcode_t err = fn (extra, node); if (BE (err != REG_NOERROR, 0)) return err; /* Go to the left node, or up and to the right. */ if (node->left) node = node->left; else { bin_tree_t *prev = NULL; while (node->right == prev || node->right == NULL) { prev = node; node = node->parent; if (!node) return REG_NOERROR; } node = node->right; } } } /* Optimization pass: if a SUBEXP is entirely contained, strip it and tell re_search_internal to map the inner one's opr.idx to this one's. Adjust backreferences as well. Requires a preorder visit. */ static reg_errcode_t optimize_subexps (void *extra, bin_tree_t *node) { re_dfa_t *dfa = (re_dfa_t *) extra; if (node->token.type == OP_BACK_REF && dfa->subexp_map) { int idx = node->token.opr.idx; node->token.opr.idx = dfa->subexp_map[idx]; dfa->used_bkref_map |= 1 << node->token.opr.idx; } else if (node->token.type == SUBEXP && node->left && node->left->token.type == SUBEXP) { Idx other_idx = node->left->token.opr.idx; node->left = node->left->left; if (node->left) node->left->parent = node; dfa->subexp_map[other_idx] = dfa->subexp_map[node->token.opr.idx]; if (other_idx < BITSET_WORD_BITS) dfa->used_bkref_map &= ~((bitset_word_t) 1 << other_idx); } return REG_NOERROR; } /* Lowering pass: Turn each SUBEXP node into the appropriate concatenation of OP_OPEN_SUBEXP, the body of the SUBEXP (if any) and OP_CLOSE_SUBEXP. */ static reg_errcode_t lower_subexps (void *extra, bin_tree_t *node) { regex_t *preg = (regex_t *) extra; reg_errcode_t err = REG_NOERROR; if (node->left && node->left->token.type == SUBEXP) { node->left = lower_subexp (&err, preg, node->left); if (node->left) node->left->parent = node; } if (node->right && node->right->token.type == SUBEXP) { node->right = lower_subexp (&err, preg, node->right); if (node->right) node->right->parent = node; } return err; } static bin_tree_t * lower_subexp (reg_errcode_t *err, regex_t *preg, bin_tree_t *node) { re_dfa_t *dfa = preg->buffer; bin_tree_t *body = node->left; bin_tree_t *op, *cls, *tree1, *tree; if (preg->no_sub /* We do not optimize empty subexpressions, because otherwise we may have bad CONCAT nodes with NULL children. This is obviously not very common, so we do not lose much. An example that triggers this case is the sed "script" /\(\)/x. */ && node->left != NULL && (node->token.opr.idx >= BITSET_WORD_BITS || !(dfa->used_bkref_map & ((bitset_word_t) 1 << node->token.opr.idx)))) return node->left; /* Convert the SUBEXP node to the concatenation of an OP_OPEN_SUBEXP, the contents, and an OP_CLOSE_SUBEXP. */ op = create_tree (dfa, NULL, NULL, OP_OPEN_SUBEXP); cls = create_tree (dfa, NULL, NULL, OP_CLOSE_SUBEXP); tree1 = body ? create_tree (dfa, body, cls, CONCAT) : cls; tree = create_tree (dfa, op, tree1, CONCAT); if (BE (tree == NULL || tree1 == NULL || op == NULL || cls == NULL, 0)) { *err = REG_ESPACE; return NULL; } op->token.opr.idx = cls->token.opr.idx = node->token.opr.idx; op->token.opt_subexp = cls->token.opt_subexp = node->token.opt_subexp; return tree; } /* Pass 1 in building the NFA: compute FIRST and create unlinked automaton nodes. Requires a postorder visit. */ static reg_errcode_t calc_first (void *extra, bin_tree_t *node) { re_dfa_t *dfa = (re_dfa_t *) extra; if (node->token.type == CONCAT) { node->first = node->left->first; node->node_idx = node->left->node_idx; } else { node->first = node; node->node_idx = re_dfa_add_node (dfa, node->token); if (BE (node->node_idx == -1, 0)) return REG_ESPACE; if (node->token.type == ANCHOR) dfa->nodes[node->node_idx].constraint = node->token.opr.ctx_type; } return REG_NOERROR; } /* Pass 2: compute NEXT on the tree. Preorder visit. */ static reg_errcode_t calc_next (void *extra, bin_tree_t *node) { switch (node->token.type) { case OP_DUP_ASTERISK: node->left->next = node; break; case CONCAT: node->left->next = node->right->first; node->right->next = node->next; break; default: if (node->left) node->left->next = node->next; if (node->right) node->right->next = node->next; break; } return REG_NOERROR; } /* Pass 3: link all DFA nodes to their NEXT node (any order will do). */ static reg_errcode_t link_nfa_nodes (void *extra, bin_tree_t *node) { re_dfa_t *dfa = (re_dfa_t *) extra; Idx idx = node->node_idx; reg_errcode_t err = REG_NOERROR; switch (node->token.type) { case CONCAT: break; case END_OF_RE: assert (node->next == NULL); break; case OP_DUP_ASTERISK: case OP_ALT: { Idx left, right; dfa->has_plural_match = 1; if (node->left != NULL) left = node->left->first->node_idx; else left = node->next->node_idx; if (node->right != NULL) right = node->right->first->node_idx; else right = node->next->node_idx; assert (left > -1); assert (right > -1); err = re_node_set_init_2 (dfa->edests + idx, left, right); } break; case ANCHOR: case OP_OPEN_SUBEXP: case OP_CLOSE_SUBEXP: err = re_node_set_init_1 (dfa->edests + idx, node->next->node_idx); break; case OP_BACK_REF: dfa->nexts[idx] = node->next->node_idx; if (node->token.type == OP_BACK_REF) err = re_node_set_init_1 (dfa->edests + idx, dfa->nexts[idx]); break; default: assert (!IS_EPSILON_NODE (node->token.type)); dfa->nexts[idx] = node->next->node_idx; break; } return err; } /* Duplicate the epsilon closure of the node ROOT_NODE. Note that duplicated nodes have constraint INIT_CONSTRAINT in addition to their own constraint. */ static reg_errcode_t internal_function duplicate_node_closure (re_dfa_t *dfa, Idx top_org_node, Idx top_clone_node, Idx root_node, unsigned int init_constraint) { Idx org_node, clone_node; bool ok; unsigned int constraint = init_constraint; for (org_node = top_org_node, clone_node = top_clone_node;;) { Idx org_dest, clone_dest; if (dfa->nodes[org_node].type == OP_BACK_REF) { /* If the back reference epsilon-transit, its destination must also have the constraint. Then duplicate the epsilon closure of the destination of the back reference, and store it in edests of the back reference. */ org_dest = dfa->nexts[org_node]; re_node_set_empty (dfa->edests + clone_node); clone_dest = duplicate_node (dfa, org_dest, constraint); if (BE (clone_dest == -1, 0)) return REG_ESPACE; dfa->nexts[clone_node] = dfa->nexts[org_node]; ok = re_node_set_insert (dfa->edests + clone_node, clone_dest); if (BE (! ok, 0)) return REG_ESPACE; } else if (dfa->edests[org_node].nelem == 0) { /* In case of the node can't epsilon-transit, don't duplicate the destination and store the original destination as the destination of the node. */ dfa->nexts[clone_node] = dfa->nexts[org_node]; break; } else if (dfa->edests[org_node].nelem == 1) { /* In case of the node can epsilon-transit, and it has only one destination. */ org_dest = dfa->edests[org_node].elems[0]; re_node_set_empty (dfa->edests + clone_node); /* If the node is root_node itself, it means the epsilon closure has a loop. Then tie it to the destination of the root_node. */ if (org_node == root_node && clone_node != org_node) { ok = re_node_set_insert (dfa->edests + clone_node, org_dest); if (BE (! ok, 0)) return REG_ESPACE; break; } /* In case the node has another constraint, append it. */ constraint |= dfa->nodes[org_node].constraint; clone_dest = duplicate_node (dfa, org_dest, constraint); if (BE (clone_dest == -1, 0)) return REG_ESPACE; ok = re_node_set_insert (dfa->edests + clone_node, clone_dest); if (BE (! ok, 0)) return REG_ESPACE; } else /* dfa->edests[org_node].nelem == 2 */ { /* In case of the node can epsilon-transit, and it has two destinations. In the bin_tree_t and DFA, that's '|' and '*'. */ org_dest = dfa->edests[org_node].elems[0]; re_node_set_empty (dfa->edests + clone_node); /* Search for a duplicated node which satisfies the constraint. */ clone_dest = search_duplicated_node (dfa, org_dest, constraint); if (clone_dest == -1) { /* There is no such duplicated node, create a new one. */ reg_errcode_t err; clone_dest = duplicate_node (dfa, org_dest, constraint); if (BE (clone_dest == -1, 0)) return REG_ESPACE; ok = re_node_set_insert (dfa->edests + clone_node, clone_dest); if (BE (! ok, 0)) return REG_ESPACE; err = duplicate_node_closure (dfa, org_dest, clone_dest, root_node, constraint); if (BE (err != REG_NOERROR, 0)) return err; } else { /* There is a duplicated node which satisfies the constraint, use it to avoid infinite loop. */ ok = re_node_set_insert (dfa->edests + clone_node, clone_dest); if (BE (! ok, 0)) return REG_ESPACE; } org_dest = dfa->edests[org_node].elems[1]; clone_dest = duplicate_node (dfa, org_dest, constraint); if (BE (clone_dest == -1, 0)) return REG_ESPACE; ok = re_node_set_insert (dfa->edests + clone_node, clone_dest); if (BE (! ok, 0)) return REG_ESPACE; } org_node = org_dest; clone_node = clone_dest; } return REG_NOERROR; } /* Search for a node which is duplicated from the node ORG_NODE, and satisfies the constraint CONSTRAINT. */ static Idx search_duplicated_node (const re_dfa_t *dfa, Idx org_node, unsigned int constraint) { Idx idx; for (idx = dfa->nodes_len - 1; dfa->nodes[idx].duplicated && idx > 0; --idx) { if (org_node == dfa->org_indices[idx] && constraint == dfa->nodes[idx].constraint) return idx; /* Found. */ } return -1; /* Not found. */ } /* Duplicate the node whose index is ORG_IDX and set the constraint CONSTRAINT. Return the index of the new node, or -1 if insufficient storage is available. */ static Idx duplicate_node (re_dfa_t *dfa, Idx org_idx, unsigned int constraint) { Idx dup_idx = re_dfa_add_node (dfa, dfa->nodes[org_idx]); if (BE (dup_idx != -1, 1)) { dfa->nodes[dup_idx].constraint = constraint; dfa->nodes[dup_idx].constraint |= dfa->nodes[org_idx].constraint; dfa->nodes[dup_idx].duplicated = 1; /* Store the index of the original node. */ dfa->org_indices[dup_idx] = org_idx; } return dup_idx; } static reg_errcode_t calc_inveclosure (re_dfa_t *dfa) { Idx src, idx; bool ok; for (idx = 0; idx < dfa->nodes_len; ++idx) re_node_set_init_empty (dfa->inveclosures + idx); for (src = 0; src < dfa->nodes_len; ++src) { Idx *elems = dfa->eclosures[src].elems; for (idx = 0; idx < dfa->eclosures[src].nelem; ++idx) { ok = re_node_set_insert_last (dfa->inveclosures + elems[idx], src); if (BE (! ok, 0)) return REG_ESPACE; } } return REG_NOERROR; } /* Calculate "eclosure" for all the node in DFA. */ static reg_errcode_t calc_eclosure (re_dfa_t *dfa) { Idx node_idx; bool incomplete; #ifdef DEBUG assert (dfa->nodes_len > 0); #endif incomplete = false; /* For each nodes, calculate epsilon closure. */ for (node_idx = 0; ; ++node_idx) { reg_errcode_t err; re_node_set eclosure_elem; if (node_idx == dfa->nodes_len) { if (!incomplete) break; incomplete = false; node_idx = 0; } #ifdef DEBUG assert (dfa->eclosures[node_idx].nelem != -1); #endif /* If we have already calculated, skip it. */ if (dfa->eclosures[node_idx].nelem != 0) continue; /* Calculate epsilon closure of 'node_idx'. */ err = calc_eclosure_iter (&eclosure_elem, dfa, node_idx, true); if (BE (err != REG_NOERROR, 0)) return err; if (dfa->eclosures[node_idx].nelem == 0) { incomplete = true; re_node_set_free (&eclosure_elem); } } return REG_NOERROR; } /* Calculate epsilon closure of NODE. */ static reg_errcode_t calc_eclosure_iter (re_node_set *new_set, re_dfa_t *dfa, Idx node, bool root) { reg_errcode_t err; Idx i; re_node_set eclosure; bool ok; bool incomplete = false; err = re_node_set_alloc (&eclosure, dfa->edests[node].nelem + 1); if (BE (err != REG_NOERROR, 0)) return err; /* This indicates that we are calculating this node now. We reference this value to avoid infinite loop. */ dfa->eclosures[node].nelem = -1; /* If the current node has constraints, duplicate all nodes since they must inherit the constraints. */ if (dfa->nodes[node].constraint && dfa->edests[node].nelem && !dfa->nodes[dfa->edests[node].elems[0]].duplicated) { err = duplicate_node_closure (dfa, node, node, node, dfa->nodes[node].constraint); if (BE (err != REG_NOERROR, 0)) return err; } /* Expand each epsilon destination nodes. */ if (IS_EPSILON_NODE(dfa->nodes[node].type)) for (i = 0; i < dfa->edests[node].nelem; ++i) { re_node_set eclosure_elem; Idx edest = dfa->edests[node].elems[i]; /* If calculating the epsilon closure of 'edest' is in progress, return intermediate result. */ if (dfa->eclosures[edest].nelem == -1) { incomplete = true; continue; } /* If we haven't calculated the epsilon closure of 'edest' yet, calculate now. Otherwise use calculated epsilon closure. */ if (dfa->eclosures[edest].nelem == 0) { err = calc_eclosure_iter (&eclosure_elem, dfa, edest, false); if (BE (err != REG_NOERROR, 0)) return err; } else eclosure_elem = dfa->eclosures[edest]; /* Merge the epsilon closure of 'edest'. */ err = re_node_set_merge (&eclosure, &eclosure_elem); if (BE (err != REG_NOERROR, 0)) return err; /* If the epsilon closure of 'edest' is incomplete, the epsilon closure of this node is also incomplete. */ if (dfa->eclosures[edest].nelem == 0) { incomplete = true; re_node_set_free (&eclosure_elem); } } /* An epsilon closure includes itself. */ ok = re_node_set_insert (&eclosure, node); if (BE (! ok, 0)) return REG_ESPACE; if (incomplete && !root) dfa->eclosures[node].nelem = 0; else dfa->eclosures[node] = eclosure; *new_set = eclosure; return REG_NOERROR; } /* Functions for token which are used in the parser. */ /* Fetch a token from INPUT. We must not use this function inside bracket expressions. */ static void internal_function fetch_token (re_token_t *result, re_string_t *input, reg_syntax_t syntax) { re_string_skip_bytes (input, peek_token (result, input, syntax)); } /* Peek a token from INPUT, and return the length of the token. We must not use this function inside bracket expressions. */ static int internal_function peek_token (re_token_t *token, re_string_t *input, reg_syntax_t syntax) { unsigned char c; if (re_string_eoi (input)) { token->type = END_OF_RE; return 0; } c = re_string_peek_byte (input, 0); token->opr.c = c; token->word_char = 0; #ifdef RE_ENABLE_I18N token->mb_partial = 0; if (input->mb_cur_max > 1 && !re_string_first_byte (input, re_string_cur_idx (input))) { token->type = CHARACTER; token->mb_partial = 1; return 1; } #endif if (c == '\\') { unsigned char c2; if (re_string_cur_idx (input) + 1 >= re_string_length (input)) { token->type = BACK_SLASH; return 1; } c2 = re_string_peek_byte_case (input, 1); token->opr.c = c2; token->type = CHARACTER; #ifdef RE_ENABLE_I18N if (input->mb_cur_max > 1) { wint_t wc = re_string_wchar_at (input, re_string_cur_idx (input) + 1); token->word_char = IS_WIDE_WORD_CHAR (wc) != 0; } else #endif token->word_char = IS_WORD_CHAR (c2) != 0; switch (c2) { case '|': if (!(syntax & RE_LIMITED_OPS) && !(syntax & RE_NO_BK_VBAR)) token->type = OP_ALT; break; case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': if (!(syntax & RE_NO_BK_REFS)) { token->type = OP_BACK_REF; token->opr.idx = c2 - '1'; } break; case '<': if (!(syntax & RE_NO_GNU_OPS)) { token->type = ANCHOR; token->opr.ctx_type = WORD_FIRST; } break; case '>': if (!(syntax & RE_NO_GNU_OPS)) { token->type = ANCHOR; token->opr.ctx_type = WORD_LAST; } break; case 'b': if (!(syntax & RE_NO_GNU_OPS)) { token->type = ANCHOR; token->opr.ctx_type = WORD_DELIM; } break; case 'B': if (!(syntax & RE_NO_GNU_OPS)) { token->type = ANCHOR; token->opr.ctx_type = NOT_WORD_DELIM; } break; case 'w': if (!(syntax & RE_NO_GNU_OPS)) token->type = OP_WORD; break; case 'W': if (!(syntax & RE_NO_GNU_OPS)) token->type = OP_NOTWORD; break; case 's': if (!(syntax & RE_NO_GNU_OPS)) token->type = OP_SPACE; break; case 'S': if (!(syntax & RE_NO_GNU_OPS)) token->type = OP_NOTSPACE; break; case '`': if (!(syntax & RE_NO_GNU_OPS)) { token->type = ANCHOR; token->opr.ctx_type = BUF_FIRST; } break; case '\'': if (!(syntax & RE_NO_GNU_OPS)) { token->type = ANCHOR; token->opr.ctx_type = BUF_LAST; } break; case '(': if (!(syntax & RE_NO_BK_PARENS)) token->type = OP_OPEN_SUBEXP; break; case ')': if (!(syntax & RE_NO_BK_PARENS)) token->type = OP_CLOSE_SUBEXP; break; case '+': if (!(syntax & RE_LIMITED_OPS) && (syntax & RE_BK_PLUS_QM)) token->type = OP_DUP_PLUS; break; case '?': if (!(syntax & RE_LIMITED_OPS) && (syntax & RE_BK_PLUS_QM)) token->type = OP_DUP_QUESTION; break; case '{': if ((syntax & RE_INTERVALS) && (!(syntax & RE_NO_BK_BRACES))) token->type = OP_OPEN_DUP_NUM; break; case '}': if ((syntax & RE_INTERVALS) && (!(syntax & RE_NO_BK_BRACES))) token->type = OP_CLOSE_DUP_NUM; break; default: break; } return 2; } token->type = CHARACTER; #ifdef RE_ENABLE_I18N if (input->mb_cur_max > 1) { wint_t wc = re_string_wchar_at (input, re_string_cur_idx (input)); token->word_char = IS_WIDE_WORD_CHAR (wc) != 0; } else #endif token->word_char = IS_WORD_CHAR (token->opr.c); switch (c) { case '\n': if (syntax & RE_NEWLINE_ALT) token->type = OP_ALT; break; case '|': if (!(syntax & RE_LIMITED_OPS) && (syntax & RE_NO_BK_VBAR)) token->type = OP_ALT; break; case '*': token->type = OP_DUP_ASTERISK; break; case '+': if (!(syntax & RE_LIMITED_OPS) && !(syntax & RE_BK_PLUS_QM)) token->type = OP_DUP_PLUS; break; case '?': if (!(syntax & RE_LIMITED_OPS) && !(syntax & RE_BK_PLUS_QM)) token->type = OP_DUP_QUESTION; break; case '{': if ((syntax & RE_INTERVALS) && (syntax & RE_NO_BK_BRACES)) token->type = OP_OPEN_DUP_NUM; break; case '}': if ((syntax & RE_INTERVALS) && (syntax & RE_NO_BK_BRACES)) token->type = OP_CLOSE_DUP_NUM; break; case '(': if (syntax & RE_NO_BK_PARENS) token->type = OP_OPEN_SUBEXP; break; case ')': if (syntax & RE_NO_BK_PARENS) token->type = OP_CLOSE_SUBEXP; break; case '[': token->type = OP_OPEN_BRACKET; break; case '.': token->type = OP_PERIOD; break; case '^': if (!(syntax & (RE_CONTEXT_INDEP_ANCHORS | RE_CARET_ANCHORS_HERE)) && re_string_cur_idx (input) != 0) { char prev = re_string_peek_byte (input, -1); if (!(syntax & RE_NEWLINE_ALT) || prev != '\n') break; } token->type = ANCHOR; token->opr.ctx_type = LINE_FIRST; break; case '$': if (!(syntax & RE_CONTEXT_INDEP_ANCHORS) && re_string_cur_idx (input) + 1 != re_string_length (input)) { re_token_t next; re_string_skip_bytes (input, 1); peek_token (&next, input, syntax); re_string_skip_bytes (input, -1); if (next.type != OP_ALT && next.type != OP_CLOSE_SUBEXP) break; } token->type = ANCHOR; token->opr.ctx_type = LINE_LAST; break; default: break; } return 1; } /* Peek a token from INPUT, and return the length of the token. We must not use this function out of bracket expressions. */ static int internal_function peek_token_bracket (re_token_t *token, re_string_t *input, reg_syntax_t syntax) { unsigned char c; if (re_string_eoi (input)) { token->type = END_OF_RE; return 0; } c = re_string_peek_byte (input, 0); token->opr.c = c; #ifdef RE_ENABLE_I18N if (input->mb_cur_max > 1 && !re_string_first_byte (input, re_string_cur_idx (input))) { token->type = CHARACTER; return 1; } #endif /* RE_ENABLE_I18N */ if (c == '\\' && (syntax & RE_BACKSLASH_ESCAPE_IN_LISTS) && re_string_cur_idx (input) + 1 < re_string_length (input)) { /* In this case, '\' escape a character. */ unsigned char c2; re_string_skip_bytes (input, 1); c2 = re_string_peek_byte (input, 0); token->opr.c = c2; token->type = CHARACTER; return 1; } if (c == '[') /* '[' is a special char in a bracket exps. */ { unsigned char c2; int token_len; if (re_string_cur_idx (input) + 1 < re_string_length (input)) c2 = re_string_peek_byte (input, 1); else c2 = 0; token->opr.c = c2; token_len = 2; switch (c2) { case '.': token->type = OP_OPEN_COLL_ELEM; break; case '=': token->type = OP_OPEN_EQUIV_CLASS; break; case ':': if (syntax & RE_CHAR_CLASSES) { token->type = OP_OPEN_CHAR_CLASS; break; } /* else fall through. */ default: token->type = CHARACTER; token->opr.c = c; token_len = 1; break; } return token_len; } switch (c) { case '-': token->type = OP_CHARSET_RANGE; break; case ']': token->type = OP_CLOSE_BRACKET; break; case '^': token->type = OP_NON_MATCH_LIST; break; default: token->type = CHARACTER; } return 1; } /* Functions for parser. */ /* Entry point of the parser. Parse the regular expression REGEXP and return the structure tree. If an error occurs, ERR is set by error code, and return NULL. This function build the following tree, from regular expression : CAT / \ / \ EOR CAT means concatenation. EOR means end of regular expression. */ static bin_tree_t * parse (re_string_t *regexp, regex_t *preg, reg_syntax_t syntax, reg_errcode_t *err) { re_dfa_t *dfa = preg->buffer; bin_tree_t *tree, *eor, *root; re_token_t current_token; dfa->syntax = syntax; fetch_token (¤t_token, regexp, syntax | RE_CARET_ANCHORS_HERE); tree = parse_reg_exp (regexp, preg, ¤t_token, syntax, 0, err); if (BE (*err != REG_NOERROR && tree == NULL, 0)) return NULL; eor = create_tree (dfa, NULL, NULL, END_OF_RE); if (tree != NULL) root = create_tree (dfa, tree, eor, CONCAT); else root = eor; if (BE (eor == NULL || root == NULL, 0)) { *err = REG_ESPACE; return NULL; } return root; } /* This function build the following tree, from regular expression |: ALT / \ / \ ALT means alternative, which represents the operator '|'. */ static bin_tree_t * parse_reg_exp (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err) { re_dfa_t *dfa = preg->buffer; bin_tree_t *tree, *branch = NULL; bitset_word_t initial_bkref_map = dfa->completed_bkref_map; tree = parse_branch (regexp, preg, token, syntax, nest, err); if (BE (*err != REG_NOERROR && tree == NULL, 0)) return NULL; while (token->type == OP_ALT) { fetch_token (token, regexp, syntax | RE_CARET_ANCHORS_HERE); if (token->type != OP_ALT && token->type != END_OF_RE && (nest == 0 || token->type != OP_CLOSE_SUBEXP)) { bitset_word_t accumulated_bkref_map = dfa->completed_bkref_map; dfa->completed_bkref_map = initial_bkref_map; branch = parse_branch (regexp, preg, token, syntax, nest, err); if (BE (*err != REG_NOERROR && branch == NULL, 0)) { if (tree != NULL) postorder (tree, free_tree, NULL); return NULL; } dfa->completed_bkref_map |= accumulated_bkref_map; } else branch = NULL; tree = create_tree (dfa, tree, branch, OP_ALT); if (BE (tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } } return tree; } /* This function build the following tree, from regular expression : CAT / \ / \ CAT means concatenation. */ static bin_tree_t * parse_branch (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err) { bin_tree_t *tree, *expr; re_dfa_t *dfa = preg->buffer; tree = parse_expression (regexp, preg, token, syntax, nest, err); if (BE (*err != REG_NOERROR && tree == NULL, 0)) return NULL; while (token->type != OP_ALT && token->type != END_OF_RE && (nest == 0 || token->type != OP_CLOSE_SUBEXP)) { expr = parse_expression (regexp, preg, token, syntax, nest, err); if (BE (*err != REG_NOERROR && expr == NULL, 0)) { if (tree != NULL) postorder (tree, free_tree, NULL); return NULL; } if (tree != NULL && expr != NULL) { bin_tree_t *newtree = create_tree (dfa, tree, expr, CONCAT); if (newtree == NULL) { postorder (expr, free_tree, NULL); postorder (tree, free_tree, NULL); *err = REG_ESPACE; return NULL; } tree = newtree; } else if (tree == NULL) tree = expr; /* Otherwise expr == NULL, we don't need to create new tree. */ } return tree; } /* This function build the following tree, from regular expression a*: * | a */ static bin_tree_t * parse_expression (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err) { re_dfa_t *dfa = preg->buffer; bin_tree_t *tree; switch (token->type) { case CHARACTER: tree = create_token_tree (dfa, NULL, NULL, token); if (BE (tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) { while (!re_string_eoi (regexp) && !re_string_first_byte (regexp, re_string_cur_idx (regexp))) { bin_tree_t *mbc_remain; fetch_token (token, regexp, syntax); mbc_remain = create_token_tree (dfa, NULL, NULL, token); tree = create_tree (dfa, tree, mbc_remain, CONCAT); if (BE (mbc_remain == NULL || tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } } } #endif break; case OP_OPEN_SUBEXP: tree = parse_sub_exp (regexp, preg, token, syntax, nest + 1, err); if (BE (*err != REG_NOERROR && tree == NULL, 0)) return NULL; break; case OP_OPEN_BRACKET: tree = parse_bracket_exp (regexp, dfa, token, syntax, err); if (BE (*err != REG_NOERROR && tree == NULL, 0)) return NULL; break; case OP_BACK_REF: if (!BE (dfa->completed_bkref_map & (1 << token->opr.idx), 1)) { *err = REG_ESUBREG; return NULL; } dfa->used_bkref_map |= 1 << token->opr.idx; tree = create_token_tree (dfa, NULL, NULL, token); if (BE (tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } ++dfa->nbackref; dfa->has_mb_node = 1; break; case OP_OPEN_DUP_NUM: if (syntax & RE_CONTEXT_INVALID_DUP) { *err = REG_BADRPT; return NULL; } /* FALLTHROUGH */ case OP_DUP_ASTERISK: case OP_DUP_PLUS: case OP_DUP_QUESTION: if (syntax & RE_CONTEXT_INVALID_OPS) { *err = REG_BADRPT; return NULL; } else if (syntax & RE_CONTEXT_INDEP_OPS) { fetch_token (token, regexp, syntax); return parse_expression (regexp, preg, token, syntax, nest, err); } /* else fall through */ case OP_CLOSE_SUBEXP: if ((token->type == OP_CLOSE_SUBEXP) && !(syntax & RE_UNMATCHED_RIGHT_PAREN_ORD)) { *err = REG_ERPAREN; return NULL; } /* else fall through */ case OP_CLOSE_DUP_NUM: /* We treat it as a normal character. */ /* Then we can these characters as normal characters. */ token->type = CHARACTER; /* mb_partial and word_char bits should be initialized already by peek_token. */ tree = create_token_tree (dfa, NULL, NULL, token); if (BE (tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } break; case ANCHOR: if ((token->opr.ctx_type & (WORD_DELIM | NOT_WORD_DELIM | WORD_FIRST | WORD_LAST)) && dfa->word_ops_used == 0) init_word_char (dfa); if (token->opr.ctx_type == WORD_DELIM || token->opr.ctx_type == NOT_WORD_DELIM) { bin_tree_t *tree_first, *tree_last; if (token->opr.ctx_type == WORD_DELIM) { token->opr.ctx_type = WORD_FIRST; tree_first = create_token_tree (dfa, NULL, NULL, token); token->opr.ctx_type = WORD_LAST; } else { token->opr.ctx_type = INSIDE_WORD; tree_first = create_token_tree (dfa, NULL, NULL, token); token->opr.ctx_type = INSIDE_NOTWORD; } tree_last = create_token_tree (dfa, NULL, NULL, token); tree = create_tree (dfa, tree_first, tree_last, OP_ALT); if (BE (tree_first == NULL || tree_last == NULL || tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } } else { tree = create_token_tree (dfa, NULL, NULL, token); if (BE (tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } } /* We must return here, since ANCHORs can't be followed by repetition operators. eg. RE"^*" is invalid or "", it must not be "". */ fetch_token (token, regexp, syntax); return tree; case OP_PERIOD: tree = create_token_tree (dfa, NULL, NULL, token); if (BE (tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } if (dfa->mb_cur_max > 1) dfa->has_mb_node = 1; break; case OP_WORD: case OP_NOTWORD: tree = build_charclass_op (dfa, regexp->trans, "alnum", "_", token->type == OP_NOTWORD, err); if (BE (*err != REG_NOERROR && tree == NULL, 0)) return NULL; break; case OP_SPACE: case OP_NOTSPACE: tree = build_charclass_op (dfa, regexp->trans, "space", "", token->type == OP_NOTSPACE, err); if (BE (*err != REG_NOERROR && tree == NULL, 0)) return NULL; break; case OP_ALT: case END_OF_RE: return NULL; case BACK_SLASH: *err = REG_EESCAPE; return NULL; default: /* Must not happen? */ #ifdef DEBUG assert (0); #endif return NULL; } fetch_token (token, regexp, syntax); while (token->type == OP_DUP_ASTERISK || token->type == OP_DUP_PLUS || token->type == OP_DUP_QUESTION || token->type == OP_OPEN_DUP_NUM) { bin_tree_t *dup_tree = parse_dup_op (tree, regexp, dfa, token, syntax, err); if (BE (*err != REG_NOERROR && dup_tree == NULL, 0)) { if (tree != NULL) postorder (tree, free_tree, NULL); return NULL; } tree = dup_tree; /* In BRE consecutive duplications are not allowed. */ if ((syntax & RE_CONTEXT_INVALID_DUP) && (token->type == OP_DUP_ASTERISK || token->type == OP_OPEN_DUP_NUM)) { if (tree != NULL) postorder (tree, free_tree, NULL); *err = REG_BADRPT; return NULL; } } return tree; } /* This function build the following tree, from regular expression (): SUBEXP | */ static bin_tree_t * parse_sub_exp (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err) { re_dfa_t *dfa = preg->buffer; bin_tree_t *tree; size_t cur_nsub; cur_nsub = preg->re_nsub++; fetch_token (token, regexp, syntax | RE_CARET_ANCHORS_HERE); /* The subexpression may be a null string. */ if (token->type == OP_CLOSE_SUBEXP) tree = NULL; else { tree = parse_reg_exp (regexp, preg, token, syntax, nest, err); if (BE (*err == REG_NOERROR && token->type != OP_CLOSE_SUBEXP, 0)) { if (tree != NULL) postorder (tree, free_tree, NULL); *err = REG_EPAREN; } if (BE (*err != REG_NOERROR, 0)) return NULL; } if (cur_nsub <= '9' - '1') dfa->completed_bkref_map |= 1 << cur_nsub; tree = create_tree (dfa, tree, NULL, SUBEXP); if (BE (tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } tree->token.opr.idx = cur_nsub; return tree; } /* This function parse repetition operators like "*", "+", "{1,3}" etc. */ static bin_tree_t * parse_dup_op (bin_tree_t *elem, re_string_t *regexp, re_dfa_t *dfa, re_token_t *token, reg_syntax_t syntax, reg_errcode_t *err) { bin_tree_t *tree = NULL, *old_tree = NULL; Idx i, start, end, start_idx = re_string_cur_idx (regexp); re_token_t start_token = *token; if (token->type == OP_OPEN_DUP_NUM) { end = 0; start = fetch_number (regexp, token, syntax); if (start == -1) { if (token->type == CHARACTER && token->opr.c == ',') start = 0; /* We treat "{,m}" as "{0,m}". */ else { *err = REG_BADBR; /* {} is invalid. */ return NULL; } } if (BE (start != -2, 1)) { /* We treat "{n}" as "{n,n}". */ end = ((token->type == OP_CLOSE_DUP_NUM) ? start : ((token->type == CHARACTER && token->opr.c == ',') ? fetch_number (regexp, token, syntax) : -2)); } if (BE (start == -2 || end == -2, 0)) { /* Invalid sequence. */ if (BE (!(syntax & RE_INVALID_INTERVAL_ORD), 0)) { if (token->type == END_OF_RE) *err = REG_EBRACE; else *err = REG_BADBR; return NULL; } /* If the syntax bit is set, rollback. */ re_string_set_index (regexp, start_idx); *token = start_token; token->type = CHARACTER; /* mb_partial and word_char bits should be already initialized by peek_token. */ return elem; } if (BE ((end != -1 && start > end) || token->type != OP_CLOSE_DUP_NUM, 0)) { /* First number greater than second. */ *err = REG_BADBR; return NULL; } if (BE (RE_DUP_MAX < (end == -1 ? start : end), 0)) { *err = REG_ESIZE; return NULL; } } else { start = (token->type == OP_DUP_PLUS) ? 1 : 0; end = (token->type == OP_DUP_QUESTION) ? 1 : -1; } fetch_token (token, regexp, syntax); if (BE (elem == NULL, 0)) return NULL; if (BE (start == 0 && end == 0, 0)) { postorder (elem, free_tree, NULL); return NULL; } /* Extract "{n,m}" to "...{0,}". */ if (BE (start > 0, 0)) { tree = elem; for (i = 2; i <= start; ++i) { elem = duplicate_tree (elem, dfa); tree = create_tree (dfa, tree, elem, CONCAT); if (BE (elem == NULL || tree == NULL, 0)) goto parse_dup_op_espace; } if (start == end) return tree; /* Duplicate ELEM before it is marked optional. */ elem = duplicate_tree (elem, dfa); if (BE (elem == NULL, 0)) goto parse_dup_op_espace; old_tree = tree; } else old_tree = NULL; if (elem->token.type == SUBEXP) { uintptr_t subidx = elem->token.opr.idx; postorder (elem, mark_opt_subexp, (void *) subidx); } tree = create_tree (dfa, elem, NULL, (end == -1 ? OP_DUP_ASTERISK : OP_ALT)); if (BE (tree == NULL, 0)) goto parse_dup_op_espace; /* From gnulib's "intprops.h": True if the arithmetic type T is signed. */ #define TYPE_SIGNED(t) (! ((t) 0 < (t) -1)) /* This loop is actually executed only when end != -1, to rewrite {0,n} as ((...?)?)?... We have already created the start+1-th copy. */ if (TYPE_SIGNED (Idx) || end != -1) for (i = start + 2; i <= end; ++i) { elem = duplicate_tree (elem, dfa); tree = create_tree (dfa, tree, elem, CONCAT); if (BE (elem == NULL || tree == NULL, 0)) goto parse_dup_op_espace; tree = create_tree (dfa, tree, NULL, OP_ALT); if (BE (tree == NULL, 0)) goto parse_dup_op_espace; } if (old_tree) tree = create_tree (dfa, old_tree, tree, CONCAT); return tree; parse_dup_op_espace: *err = REG_ESPACE; return NULL; } /* Size of the names for collating symbol/equivalence_class/character_class. I'm not sure, but maybe enough. */ #define BRACKET_NAME_BUF_SIZE 32 #ifndef _LIBC # ifdef RE_ENABLE_I18N /* Convert the byte B to the corresponding wide character. In a unibyte locale, treat B as itself if it is an encoding error. In a multibyte locale, return WEOF if B is an encoding error. */ static wint_t parse_byte (unsigned char b, re_charset_t *mbcset) { wint_t wc = __btowc (b); return wc == WEOF && !mbcset ? b : wc; } #endif /* Local function for parse_bracket_exp only used in case of NOT _LIBC. Build the range expression which starts from START_ELEM, and ends at END_ELEM. The result are written to MBCSET and SBCSET. RANGE_ALLOC is the allocated size of mbcset->range_starts, and mbcset->range_ends, is a pointer argument since we may update it. */ static reg_errcode_t internal_function # ifdef RE_ENABLE_I18N build_range_exp (const reg_syntax_t syntax, bitset_t sbcset, re_charset_t *mbcset, Idx *range_alloc, const bracket_elem_t *start_elem, const bracket_elem_t *end_elem) # else /* not RE_ENABLE_I18N */ build_range_exp (const reg_syntax_t syntax, bitset_t sbcset, const bracket_elem_t *start_elem, const bracket_elem_t *end_elem) # endif /* not RE_ENABLE_I18N */ { unsigned int start_ch, end_ch; /* Equivalence Classes and Character Classes can't be a range start/end. */ if (BE (start_elem->type == EQUIV_CLASS || start_elem->type == CHAR_CLASS || end_elem->type == EQUIV_CLASS || end_elem->type == CHAR_CLASS, 0)) return REG_ERANGE; /* We can handle no multi character collating elements without libc support. */ if (BE ((start_elem->type == COLL_SYM && strlen ((char *) start_elem->opr.name) > 1) || (end_elem->type == COLL_SYM && strlen ((char *) end_elem->opr.name) > 1), 0)) return REG_ECOLLATE; # ifdef RE_ENABLE_I18N { wchar_t wc; wint_t start_wc; wint_t end_wc; start_ch = ((start_elem->type == SB_CHAR) ? start_elem->opr.ch : ((start_elem->type == COLL_SYM) ? start_elem->opr.name[0] : 0)); end_ch = ((end_elem->type == SB_CHAR) ? end_elem->opr.ch : ((end_elem->type == COLL_SYM) ? end_elem->opr.name[0] : 0)); start_wc = ((start_elem->type == SB_CHAR || start_elem->type == COLL_SYM) ? parse_byte (start_ch, mbcset) : start_elem->opr.wch); end_wc = ((end_elem->type == SB_CHAR || end_elem->type == COLL_SYM) ? parse_byte (end_ch, mbcset) : end_elem->opr.wch); if (start_wc == WEOF || end_wc == WEOF) return REG_ECOLLATE; else if (BE ((syntax & RE_NO_EMPTY_RANGES) && start_wc > end_wc, 0)) return REG_ERANGE; /* Got valid collation sequence values, add them as a new entry. However, for !_LIBC we have no collation elements: if the character set is single byte, the single byte character set that we build below suffices. parse_bracket_exp passes no MBCSET if dfa->mb_cur_max == 1. */ if (mbcset) { /* Check the space of the arrays. */ if (BE (*range_alloc == mbcset->nranges, 0)) { /* There is not enough space, need realloc. */ wchar_t *new_array_start, *new_array_end; Idx new_nranges; /* +1 in case of mbcset->nranges is 0. */ new_nranges = 2 * mbcset->nranges + 1; /* Use realloc since mbcset->range_starts and mbcset->range_ends are NULL if *range_alloc == 0. */ new_array_start = re_realloc (mbcset->range_starts, wchar_t, new_nranges); new_array_end = re_realloc (mbcset->range_ends, wchar_t, new_nranges); if (BE (new_array_start == NULL || new_array_end == NULL, 0)) { re_free (new_array_start); re_free (new_array_end); return REG_ESPACE; } mbcset->range_starts = new_array_start; mbcset->range_ends = new_array_end; *range_alloc = new_nranges; } mbcset->range_starts[mbcset->nranges] = start_wc; mbcset->range_ends[mbcset->nranges++] = end_wc; } /* Build the table for single byte characters. */ for (wc = 0; wc < SBC_MAX; ++wc) { if (start_wc <= wc && wc <= end_wc) bitset_set (sbcset, wc); } } # else /* not RE_ENABLE_I18N */ { unsigned int ch; start_ch = ((start_elem->type == SB_CHAR ) ? start_elem->opr.ch : ((start_elem->type == COLL_SYM) ? start_elem->opr.name[0] : 0)); end_ch = ((end_elem->type == SB_CHAR ) ? end_elem->opr.ch : ((end_elem->type == COLL_SYM) ? end_elem->opr.name[0] : 0)); if (start_ch > end_ch) return REG_ERANGE; /* Build the table for single byte characters. */ for (ch = 0; ch < SBC_MAX; ++ch) if (start_ch <= ch && ch <= end_ch) bitset_set (sbcset, ch); } # endif /* not RE_ENABLE_I18N */ return REG_NOERROR; } #endif /* not _LIBC */ #ifndef _LIBC /* Helper function for parse_bracket_exp only used in case of NOT _LIBC.. Build the collating element which is represented by NAME. The result are written to MBCSET and SBCSET. COLL_SYM_ALLOC is the allocated size of mbcset->coll_sym, is a pointer argument since we may update it. */ static reg_errcode_t internal_function # ifdef RE_ENABLE_I18N build_collating_symbol (bitset_t sbcset, re_charset_t *mbcset, Idx *coll_sym_alloc, const unsigned char *name) # else /* not RE_ENABLE_I18N */ build_collating_symbol (bitset_t sbcset, const unsigned char *name) # endif /* not RE_ENABLE_I18N */ { size_t name_len = strlen ((const char *) name); if (BE (name_len != 1, 0)) return REG_ECOLLATE; else { bitset_set (sbcset, name[0]); return REG_NOERROR; } } #endif /* not _LIBC */ /* This function parse bracket expression like "[abc]", "[a-c]", "[[.a-a.]]" etc. */ static bin_tree_t * parse_bracket_exp (re_string_t *regexp, re_dfa_t *dfa, re_token_t *token, reg_syntax_t syntax, reg_errcode_t *err) { #ifdef _LIBC const unsigned char *collseqmb; const char *collseqwc; uint32_t nrules; int32_t table_size; const int32_t *symb_table; const unsigned char *extra; /* Local function for parse_bracket_exp used in _LIBC environment. Seek the collating symbol entry corresponding to NAME. Return the index of the symbol in the SYMB_TABLE, or -1 if not found. */ auto inline int32_t __attribute__ ((always_inline)) seek_collating_symbol_entry (const unsigned char *name, size_t name_len) { int32_t elem; for (elem = 0; elem < table_size; elem++) if (symb_table[2 * elem] != 0) { int32_t idx = symb_table[2 * elem + 1]; /* Skip the name of collating element name. */ idx += 1 + extra[idx]; if (/* Compare the length of the name. */ name_len == extra[idx] /* Compare the name. */ && memcmp (name, &extra[idx + 1], name_len) == 0) /* Yep, this is the entry. */ return elem; } return -1; } /* Local function for parse_bracket_exp used in _LIBC environment. Look up the collation sequence value of BR_ELEM. Return the value if succeeded, UINT_MAX otherwise. */ auto inline unsigned int __attribute__ ((always_inline)) lookup_collation_sequence_value (bracket_elem_t *br_elem) { if (br_elem->type == SB_CHAR) { /* if (MB_CUR_MAX == 1) */ if (nrules == 0) return collseqmb[br_elem->opr.ch]; else { wint_t wc = __btowc (br_elem->opr.ch); return __collseq_table_lookup (collseqwc, wc); } } else if (br_elem->type == MB_CHAR) { if (nrules != 0) return __collseq_table_lookup (collseqwc, br_elem->opr.wch); } else if (br_elem->type == COLL_SYM) { size_t sym_name_len = strlen ((char *) br_elem->opr.name); if (nrules != 0) { int32_t elem, idx; elem = seek_collating_symbol_entry (br_elem->opr.name, sym_name_len); if (elem != -1) { /* We found the entry. */ idx = symb_table[2 * elem + 1]; /* Skip the name of collating element name. */ idx += 1 + extra[idx]; /* Skip the byte sequence of the collating element. */ idx += 1 + extra[idx]; /* Adjust for the alignment. */ idx = (idx + 3) & ~3; /* Skip the multibyte collation sequence value. */ idx += sizeof (unsigned int); /* Skip the wide char sequence of the collating element. */ idx += sizeof (unsigned int) * (1 + *(unsigned int *) (extra + idx)); /* Return the collation sequence value. */ return *(unsigned int *) (extra + idx); } else if (sym_name_len == 1) { /* No valid character. Match it as a single byte character. */ return collseqmb[br_elem->opr.name[0]]; } } else if (sym_name_len == 1) return collseqmb[br_elem->opr.name[0]]; } return UINT_MAX; } /* Local function for parse_bracket_exp used in _LIBC environment. Build the range expression which starts from START_ELEM, and ends at END_ELEM. The result are written to MBCSET and SBCSET. RANGE_ALLOC is the allocated size of mbcset->range_starts, and mbcset->range_ends, is a pointer argument since we may update it. */ auto inline reg_errcode_t __attribute__ ((always_inline)) build_range_exp (bitset_t sbcset, re_charset_t *mbcset, int *range_alloc, bracket_elem_t *start_elem, bracket_elem_t *end_elem) { unsigned int ch; uint32_t start_collseq; uint32_t end_collseq; /* Equivalence Classes and Character Classes can't be a range start/end. */ if (BE (start_elem->type == EQUIV_CLASS || start_elem->type == CHAR_CLASS || end_elem->type == EQUIV_CLASS || end_elem->type == CHAR_CLASS, 0)) return REG_ERANGE; /* FIXME: Implement rational ranges here, too. */ start_collseq = lookup_collation_sequence_value (start_elem); end_collseq = lookup_collation_sequence_value (end_elem); /* Check start/end collation sequence values. */ if (BE (start_collseq == UINT_MAX || end_collseq == UINT_MAX, 0)) return REG_ECOLLATE; if (BE ((syntax & RE_NO_EMPTY_RANGES) && start_collseq > end_collseq, 0)) return REG_ERANGE; /* Got valid collation sequence values, add them as a new entry. However, if we have no collation elements, and the character set is single byte, the single byte character set that we build below suffices. */ if (nrules > 0 || dfa->mb_cur_max > 1) { /* Check the space of the arrays. */ if (BE (*range_alloc == mbcset->nranges, 0)) { /* There is not enough space, need realloc. */ uint32_t *new_array_start; uint32_t *new_array_end; Idx new_nranges; /* +1 in case of mbcset->nranges is 0. */ new_nranges = 2 * mbcset->nranges + 1; new_array_start = re_realloc (mbcset->range_starts, uint32_t, new_nranges); new_array_end = re_realloc (mbcset->range_ends, uint32_t, new_nranges); if (BE (new_array_start == NULL || new_array_end == NULL, 0)) return REG_ESPACE; mbcset->range_starts = new_array_start; mbcset->range_ends = new_array_end; *range_alloc = new_nranges; } mbcset->range_starts[mbcset->nranges] = start_collseq; mbcset->range_ends[mbcset->nranges++] = end_collseq; } /* Build the table for single byte characters. */ for (ch = 0; ch < SBC_MAX; ch++) { uint32_t ch_collseq; /* if (MB_CUR_MAX == 1) */ if (nrules == 0) ch_collseq = collseqmb[ch]; else ch_collseq = __collseq_table_lookup (collseqwc, __btowc (ch)); if (start_collseq <= ch_collseq && ch_collseq <= end_collseq) bitset_set (sbcset, ch); } return REG_NOERROR; } /* Local function for parse_bracket_exp used in _LIBC environment. Build the collating element which is represented by NAME. The result are written to MBCSET and SBCSET. COLL_SYM_ALLOC is the allocated size of mbcset->coll_sym, is a pointer argument since we may update it. */ auto inline reg_errcode_t __attribute__ ((always_inline)) build_collating_symbol (bitset_t sbcset, re_charset_t *mbcset, Idx *coll_sym_alloc, const unsigned char *name) { int32_t elem, idx; size_t name_len = strlen ((const char *) name); if (nrules != 0) { elem = seek_collating_symbol_entry (name, name_len); if (elem != -1) { /* We found the entry. */ idx = symb_table[2 * elem + 1]; /* Skip the name of collating element name. */ idx += 1 + extra[idx]; } else if (name_len == 1) { /* No valid character, treat it as a normal character. */ bitset_set (sbcset, name[0]); return REG_NOERROR; } else return REG_ECOLLATE; /* Got valid collation sequence, add it as a new entry. */ /* Check the space of the arrays. */ if (BE (*coll_sym_alloc == mbcset->ncoll_syms, 0)) { /* Not enough, realloc it. */ /* +1 in case of mbcset->ncoll_syms is 0. */ Idx new_coll_sym_alloc = 2 * mbcset->ncoll_syms + 1; /* Use realloc since mbcset->coll_syms is NULL if *alloc == 0. */ int32_t *new_coll_syms = re_realloc (mbcset->coll_syms, int32_t, new_coll_sym_alloc); if (BE (new_coll_syms == NULL, 0)) return REG_ESPACE; mbcset->coll_syms = new_coll_syms; *coll_sym_alloc = new_coll_sym_alloc; } mbcset->coll_syms[mbcset->ncoll_syms++] = idx; return REG_NOERROR; } else { if (BE (name_len != 1, 0)) return REG_ECOLLATE; else { bitset_set (sbcset, name[0]); return REG_NOERROR; } } } #endif re_token_t br_token; re_bitset_ptr_t sbcset; #ifdef RE_ENABLE_I18N re_charset_t *mbcset; Idx coll_sym_alloc = 0, range_alloc = 0, mbchar_alloc = 0; Idx equiv_class_alloc = 0, char_class_alloc = 0; #endif /* not RE_ENABLE_I18N */ bool non_match = false; bin_tree_t *work_tree; int token_len; bool first_round = true; #ifdef _LIBC collseqmb = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_COLLSEQMB); nrules = _NL_CURRENT_WORD (LC_COLLATE, _NL_COLLATE_NRULES); if (nrules) { /* if (MB_CUR_MAX > 1) */ collseqwc = _NL_CURRENT (LC_COLLATE, _NL_COLLATE_COLLSEQWC); table_size = _NL_CURRENT_WORD (LC_COLLATE, _NL_COLLATE_SYMB_HASH_SIZEMB); symb_table = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_SYMB_TABLEMB); extra = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_SYMB_EXTRAMB); } #endif sbcset = (re_bitset_ptr_t) calloc (sizeof (bitset_t), 1); #ifdef RE_ENABLE_I18N mbcset = (re_charset_t *) calloc (sizeof (re_charset_t), 1); #endif /* RE_ENABLE_I18N */ #ifdef RE_ENABLE_I18N if (BE (sbcset == NULL || mbcset == NULL, 0)) #else if (BE (sbcset == NULL, 0)) #endif /* RE_ENABLE_I18N */ { re_free (sbcset); #ifdef RE_ENABLE_I18N re_free (mbcset); #endif *err = REG_ESPACE; return NULL; } token_len = peek_token_bracket (token, regexp, syntax); if (BE (token->type == END_OF_RE, 0)) { *err = REG_BADPAT; goto parse_bracket_exp_free_return; } if (token->type == OP_NON_MATCH_LIST) { #ifdef RE_ENABLE_I18N mbcset->non_match = 1; #endif /* not RE_ENABLE_I18N */ non_match = true; if (syntax & RE_HAT_LISTS_NOT_NEWLINE) bitset_set (sbcset, '\n'); re_string_skip_bytes (regexp, token_len); /* Skip a token. */ token_len = peek_token_bracket (token, regexp, syntax); if (BE (token->type == END_OF_RE, 0)) { *err = REG_BADPAT; goto parse_bracket_exp_free_return; } } /* We treat the first ']' as a normal character. */ if (token->type == OP_CLOSE_BRACKET) token->type = CHARACTER; while (1) { bracket_elem_t start_elem, end_elem; unsigned char start_name_buf[BRACKET_NAME_BUF_SIZE]; unsigned char end_name_buf[BRACKET_NAME_BUF_SIZE]; reg_errcode_t ret; int token_len2 = 0; bool is_range_exp = false; re_token_t token2; start_elem.opr.name = start_name_buf; start_elem.type = COLL_SYM; ret = parse_bracket_element (&start_elem, regexp, token, token_len, dfa, syntax, first_round); if (BE (ret != REG_NOERROR, 0)) { *err = ret; goto parse_bracket_exp_free_return; } first_round = false; /* Get information about the next token. We need it in any case. */ token_len = peek_token_bracket (token, regexp, syntax); /* Do not check for ranges if we know they are not allowed. */ if (start_elem.type != CHAR_CLASS && start_elem.type != EQUIV_CLASS) { if (BE (token->type == END_OF_RE, 0)) { *err = REG_EBRACK; goto parse_bracket_exp_free_return; } if (token->type == OP_CHARSET_RANGE) { re_string_skip_bytes (regexp, token_len); /* Skip '-'. */ token_len2 = peek_token_bracket (&token2, regexp, syntax); if (BE (token2.type == END_OF_RE, 0)) { *err = REG_EBRACK; goto parse_bracket_exp_free_return; } if (token2.type == OP_CLOSE_BRACKET) { /* We treat the last '-' as a normal character. */ re_string_skip_bytes (regexp, -token_len); token->type = CHARACTER; } else is_range_exp = true; } } if (is_range_exp == true) { end_elem.opr.name = end_name_buf; end_elem.type = COLL_SYM; ret = parse_bracket_element (&end_elem, regexp, &token2, token_len2, dfa, syntax, true); if (BE (ret != REG_NOERROR, 0)) { *err = ret; goto parse_bracket_exp_free_return; } token_len = peek_token_bracket (token, regexp, syntax); #ifdef _LIBC *err = build_range_exp (sbcset, mbcset, &range_alloc, &start_elem, &end_elem); #else # ifdef RE_ENABLE_I18N *err = build_range_exp (syntax, sbcset, dfa->mb_cur_max > 1 ? mbcset : NULL, &range_alloc, &start_elem, &end_elem); # else *err = build_range_exp (syntax, sbcset, &start_elem, &end_elem); # endif #endif /* RE_ENABLE_I18N */ if (BE (*err != REG_NOERROR, 0)) goto parse_bracket_exp_free_return; } else { switch (start_elem.type) { case SB_CHAR: bitset_set (sbcset, start_elem.opr.ch); break; #ifdef RE_ENABLE_I18N case MB_CHAR: /* Check whether the array has enough space. */ if (BE (mbchar_alloc == mbcset->nmbchars, 0)) { wchar_t *new_mbchars; /* Not enough, realloc it. */ /* +1 in case of mbcset->nmbchars is 0. */ mbchar_alloc = 2 * mbcset->nmbchars + 1; /* Use realloc since array is NULL if *alloc == 0. */ new_mbchars = re_realloc (mbcset->mbchars, wchar_t, mbchar_alloc); if (BE (new_mbchars == NULL, 0)) goto parse_bracket_exp_espace; mbcset->mbchars = new_mbchars; } mbcset->mbchars[mbcset->nmbchars++] = start_elem.opr.wch; break; #endif /* RE_ENABLE_I18N */ case EQUIV_CLASS: *err = build_equiv_class (sbcset, #ifdef RE_ENABLE_I18N mbcset, &equiv_class_alloc, #endif /* RE_ENABLE_I18N */ start_elem.opr.name); if (BE (*err != REG_NOERROR, 0)) goto parse_bracket_exp_free_return; break; case COLL_SYM: *err = build_collating_symbol (sbcset, #ifdef RE_ENABLE_I18N mbcset, &coll_sym_alloc, #endif /* RE_ENABLE_I18N */ start_elem.opr.name); if (BE (*err != REG_NOERROR, 0)) goto parse_bracket_exp_free_return; break; case CHAR_CLASS: *err = build_charclass (regexp->trans, sbcset, #ifdef RE_ENABLE_I18N mbcset, &char_class_alloc, #endif /* RE_ENABLE_I18N */ (const char *) start_elem.opr.name, syntax); if (BE (*err != REG_NOERROR, 0)) goto parse_bracket_exp_free_return; break; default: assert (0); break; } } if (BE (token->type == END_OF_RE, 0)) { *err = REG_EBRACK; goto parse_bracket_exp_free_return; } if (token->type == OP_CLOSE_BRACKET) break; } re_string_skip_bytes (regexp, token_len); /* Skip a token. */ /* If it is non-matching list. */ if (non_match) bitset_not (sbcset); #ifdef RE_ENABLE_I18N /* Ensure only single byte characters are set. */ if (dfa->mb_cur_max > 1) bitset_mask (sbcset, dfa->sb_char); if (mbcset->nmbchars || mbcset->ncoll_syms || mbcset->nequiv_classes || mbcset->nranges || (dfa->mb_cur_max > 1 && (mbcset->nchar_classes || mbcset->non_match))) { bin_tree_t *mbc_tree; int sbc_idx; /* Build a tree for complex bracket. */ dfa->has_mb_node = 1; br_token.type = COMPLEX_BRACKET; br_token.opr.mbcset = mbcset; mbc_tree = create_token_tree (dfa, NULL, NULL, &br_token); if (BE (mbc_tree == NULL, 0)) goto parse_bracket_exp_espace; for (sbc_idx = 0; sbc_idx < BITSET_WORDS; ++sbc_idx) if (sbcset[sbc_idx]) break; /* If there are no bits set in sbcset, there is no point of having both SIMPLE_BRACKET and COMPLEX_BRACKET. */ if (sbc_idx < BITSET_WORDS) { /* Build a tree for simple bracket. */ br_token.type = SIMPLE_BRACKET; br_token.opr.sbcset = sbcset; work_tree = create_token_tree (dfa, NULL, NULL, &br_token); if (BE (work_tree == NULL, 0)) goto parse_bracket_exp_espace; /* Then join them by ALT node. */ work_tree = create_tree (dfa, work_tree, mbc_tree, OP_ALT); if (BE (work_tree == NULL, 0)) goto parse_bracket_exp_espace; } else { re_free (sbcset); work_tree = mbc_tree; } } else #endif /* not RE_ENABLE_I18N */ { #ifdef RE_ENABLE_I18N free_charset (mbcset); #endif /* Build a tree for simple bracket. */ br_token.type = SIMPLE_BRACKET; br_token.opr.sbcset = sbcset; work_tree = create_token_tree (dfa, NULL, NULL, &br_token); if (BE (work_tree == NULL, 0)) goto parse_bracket_exp_espace; } return work_tree; parse_bracket_exp_espace: *err = REG_ESPACE; parse_bracket_exp_free_return: re_free (sbcset); #ifdef RE_ENABLE_I18N free_charset (mbcset); #endif /* RE_ENABLE_I18N */ return NULL; } /* Parse an element in the bracket expression. */ static reg_errcode_t parse_bracket_element (bracket_elem_t *elem, re_string_t *regexp, re_token_t *token, int token_len, re_dfa_t *dfa, reg_syntax_t syntax, bool accept_hyphen) { #ifdef RE_ENABLE_I18N int cur_char_size; cur_char_size = re_string_char_size_at (regexp, re_string_cur_idx (regexp)); if (cur_char_size > 1) { elem->type = MB_CHAR; elem->opr.wch = re_string_wchar_at (regexp, re_string_cur_idx (regexp)); re_string_skip_bytes (regexp, cur_char_size); return REG_NOERROR; } #endif /* RE_ENABLE_I18N */ re_string_skip_bytes (regexp, token_len); /* Skip a token. */ if (token->type == OP_OPEN_COLL_ELEM || token->type == OP_OPEN_CHAR_CLASS || token->type == OP_OPEN_EQUIV_CLASS) return parse_bracket_symbol (elem, regexp, token); if (BE (token->type == OP_CHARSET_RANGE, 0) && !accept_hyphen) { /* A '-' must only appear as anything but a range indicator before the closing bracket. Everything else is an error. */ re_token_t token2; (void) peek_token_bracket (&token2, regexp, syntax); if (token2.type != OP_CLOSE_BRACKET) /* The actual error value is not standardized since this whole case is undefined. But ERANGE makes good sense. */ return REG_ERANGE; } elem->type = SB_CHAR; elem->opr.ch = token->opr.c; return REG_NOERROR; } /* Parse a bracket symbol in the bracket expression. Bracket symbols are such as [::], [..], and [==]. */ static reg_errcode_t parse_bracket_symbol (bracket_elem_t *elem, re_string_t *regexp, re_token_t *token) { unsigned char ch, delim = token->opr.c; int i = 0; if (re_string_eoi(regexp)) return REG_EBRACK; for (;; ++i) { if (i >= BRACKET_NAME_BUF_SIZE) return REG_EBRACK; if (token->type == OP_OPEN_CHAR_CLASS) ch = re_string_fetch_byte_case (regexp); else ch = re_string_fetch_byte (regexp); if (re_string_eoi(regexp)) return REG_EBRACK; if (ch == delim && re_string_peek_byte (regexp, 0) == ']') break; elem->opr.name[i] = ch; } re_string_skip_bytes (regexp, 1); elem->opr.name[i] = '\0'; switch (token->type) { case OP_OPEN_COLL_ELEM: elem->type = COLL_SYM; break; case OP_OPEN_EQUIV_CLASS: elem->type = EQUIV_CLASS; break; case OP_OPEN_CHAR_CLASS: elem->type = CHAR_CLASS; break; default: break; } return REG_NOERROR; } /* Helper function for parse_bracket_exp. Build the equivalence class which is represented by NAME. The result are written to MBCSET and SBCSET. EQUIV_CLASS_ALLOC is the allocated size of mbcset->equiv_classes, is a pointer argument since we may update it. */ static reg_errcode_t #ifdef RE_ENABLE_I18N build_equiv_class (bitset_t sbcset, re_charset_t *mbcset, Idx *equiv_class_alloc, const unsigned char *name) #else /* not RE_ENABLE_I18N */ build_equiv_class (bitset_t sbcset, const unsigned char *name) #endif /* not RE_ENABLE_I18N */ { #ifdef _LIBC uint32_t nrules = _NL_CURRENT_WORD (LC_COLLATE, _NL_COLLATE_NRULES); if (nrules != 0) { const int32_t *table, *indirect; const unsigned char *weights, *extra, *cp; unsigned char char_buf[2]; int32_t idx1, idx2; unsigned int ch; size_t len; /* Calculate the index for equivalence class. */ cp = name; table = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_TABLEMB); weights = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_WEIGHTMB); extra = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_EXTRAMB); indirect = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_INDIRECTMB); idx1 = findidx (table, indirect, extra, &cp, -1); if (BE (idx1 == 0 || *cp != '\0', 0)) /* This isn't a valid character. */ return REG_ECOLLATE; /* Build single byte matching table for this equivalence class. */ len = weights[idx1 & 0xffffff]; for (ch = 0; ch < SBC_MAX; ++ch) { char_buf[0] = ch; cp = char_buf; idx2 = findidx (table, indirect, extra, &cp, 1); /* idx2 = table[ch]; */ if (idx2 == 0) /* This isn't a valid character. */ continue; /* Compare only if the length matches and the collation rule index is the same. */ if (len == weights[idx2 & 0xffffff] && (idx1 >> 24) == (idx2 >> 24)) { int cnt = 0; while (cnt <= len && weights[(idx1 & 0xffffff) + 1 + cnt] == weights[(idx2 & 0xffffff) + 1 + cnt]) ++cnt; if (cnt > len) bitset_set (sbcset, ch); } } /* Check whether the array has enough space. */ if (BE (*equiv_class_alloc == mbcset->nequiv_classes, 0)) { /* Not enough, realloc it. */ /* +1 in case of mbcset->nequiv_classes is 0. */ Idx new_equiv_class_alloc = 2 * mbcset->nequiv_classes + 1; /* Use realloc since the array is NULL if *alloc == 0. */ int32_t *new_equiv_classes = re_realloc (mbcset->equiv_classes, int32_t, new_equiv_class_alloc); if (BE (new_equiv_classes == NULL, 0)) return REG_ESPACE; mbcset->equiv_classes = new_equiv_classes; *equiv_class_alloc = new_equiv_class_alloc; } mbcset->equiv_classes[mbcset->nequiv_classes++] = idx1; } else #endif /* _LIBC */ { if (BE (strlen ((const char *) name) != 1, 0)) return REG_ECOLLATE; bitset_set (sbcset, *name); } return REG_NOERROR; } /* Helper function for parse_bracket_exp. Build the character class which is represented by NAME. The result are written to MBCSET and SBCSET. CHAR_CLASS_ALLOC is the allocated size of mbcset->char_classes, is a pointer argument since we may update it. */ static reg_errcode_t #ifdef RE_ENABLE_I18N build_charclass (RE_TRANSLATE_TYPE trans, bitset_t sbcset, re_charset_t *mbcset, Idx *char_class_alloc, const char *class_name, reg_syntax_t syntax) #else /* not RE_ENABLE_I18N */ build_charclass (RE_TRANSLATE_TYPE trans, bitset_t sbcset, const char *class_name, reg_syntax_t syntax) #endif /* not RE_ENABLE_I18N */ { int i; const char *name = class_name; /* In case of REG_ICASE "upper" and "lower" match the both of upper and lower cases. */ if ((syntax & RE_ICASE) && (strcmp (name, "upper") == 0 || strcmp (name, "lower") == 0)) name = "alpha"; #ifdef RE_ENABLE_I18N /* Check the space of the arrays. */ if (BE (*char_class_alloc == mbcset->nchar_classes, 0)) { /* Not enough, realloc it. */ /* +1 in case of mbcset->nchar_classes is 0. */ Idx new_char_class_alloc = 2 * mbcset->nchar_classes + 1; /* Use realloc since array is NULL if *alloc == 0. */ wctype_t *new_char_classes = re_realloc (mbcset->char_classes, wctype_t, new_char_class_alloc); if (BE (new_char_classes == NULL, 0)) return REG_ESPACE; mbcset->char_classes = new_char_classes; *char_class_alloc = new_char_class_alloc; } mbcset->char_classes[mbcset->nchar_classes++] = __wctype (name); #endif /* RE_ENABLE_I18N */ #define BUILD_CHARCLASS_LOOP(ctype_func) \ do { \ if (BE (trans != NULL, 0)) \ { \ for (i = 0; i < SBC_MAX; ++i) \ if (ctype_func (i)) \ bitset_set (sbcset, trans[i]); \ } \ else \ { \ for (i = 0; i < SBC_MAX; ++i) \ if (ctype_func (i)) \ bitset_set (sbcset, i); \ } \ } while (0) if (strcmp (name, "alnum") == 0) BUILD_CHARCLASS_LOOP (isalnum); else if (strcmp (name, "cntrl") == 0) BUILD_CHARCLASS_LOOP (iscntrl); else if (strcmp (name, "lower") == 0) BUILD_CHARCLASS_LOOP (islower); else if (strcmp (name, "space") == 0) BUILD_CHARCLASS_LOOP (isspace); else if (strcmp (name, "alpha") == 0) BUILD_CHARCLASS_LOOP (isalpha); else if (strcmp (name, "digit") == 0) BUILD_CHARCLASS_LOOP (isdigit); else if (strcmp (name, "print") == 0) BUILD_CHARCLASS_LOOP (isprint); else if (strcmp (name, "upper") == 0) BUILD_CHARCLASS_LOOP (isupper); else if (strcmp (name, "blank") == 0) BUILD_CHARCLASS_LOOP (isblank); else if (strcmp (name, "graph") == 0) BUILD_CHARCLASS_LOOP (isgraph); else if (strcmp (name, "punct") == 0) BUILD_CHARCLASS_LOOP (ispunct); else if (strcmp (name, "xdigit") == 0) BUILD_CHARCLASS_LOOP (isxdigit); else return REG_ECTYPE; return REG_NOERROR; } static bin_tree_t * build_charclass_op (re_dfa_t *dfa, RE_TRANSLATE_TYPE trans, const char *class_name, const char *extra, bool non_match, reg_errcode_t *err) { re_bitset_ptr_t sbcset; #ifdef RE_ENABLE_I18N re_charset_t *mbcset; Idx alloc = 0; #endif /* not RE_ENABLE_I18N */ reg_errcode_t ret; re_token_t br_token; bin_tree_t *tree; sbcset = (re_bitset_ptr_t) calloc (sizeof (bitset_t), 1); if (BE (sbcset == NULL, 0)) { *err = REG_ESPACE; return NULL; } #ifdef RE_ENABLE_I18N mbcset = (re_charset_t *) calloc (sizeof (re_charset_t), 1); if (BE (mbcset == NULL, 0)) { re_free (sbcset); *err = REG_ESPACE; return NULL; } mbcset->non_match = non_match; #endif /* RE_ENABLE_I18N */ /* We don't care the syntax in this case. */ ret = build_charclass (trans, sbcset, #ifdef RE_ENABLE_I18N mbcset, &alloc, #endif /* RE_ENABLE_I18N */ class_name, 0); if (BE (ret != REG_NOERROR, 0)) { re_free (sbcset); #ifdef RE_ENABLE_I18N free_charset (mbcset); #endif /* RE_ENABLE_I18N */ *err = ret; return NULL; } /* \w match '_' also. */ for (; *extra; extra++) bitset_set (sbcset, *extra); /* If it is non-matching list. */ if (non_match) bitset_not (sbcset); #ifdef RE_ENABLE_I18N /* Ensure only single byte characters are set. */ if (dfa->mb_cur_max > 1) bitset_mask (sbcset, dfa->sb_char); #endif /* Build a tree for simple bracket. */ #if defined GCC_LINT || defined lint memset (&br_token, 0, sizeof br_token); #endif br_token.type = SIMPLE_BRACKET; br_token.opr.sbcset = sbcset; tree = create_token_tree (dfa, NULL, NULL, &br_token); if (BE (tree == NULL, 0)) goto build_word_op_espace; #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) { bin_tree_t *mbc_tree; /* Build a tree for complex bracket. */ br_token.type = COMPLEX_BRACKET; br_token.opr.mbcset = mbcset; dfa->has_mb_node = 1; mbc_tree = create_token_tree (dfa, NULL, NULL, &br_token); if (BE (mbc_tree == NULL, 0)) goto build_word_op_espace; /* Then join them by ALT node. */ tree = create_tree (dfa, tree, mbc_tree, OP_ALT); if (BE (mbc_tree != NULL, 1)) return tree; } else { free_charset (mbcset); return tree; } #else /* not RE_ENABLE_I18N */ return tree; #endif /* not RE_ENABLE_I18N */ build_word_op_espace: re_free (sbcset); #ifdef RE_ENABLE_I18N free_charset (mbcset); #endif /* RE_ENABLE_I18N */ *err = REG_ESPACE; return NULL; } /* This is intended for the expressions like "a{1,3}". Fetch a number from 'input', and return the number. Return -1 if the number field is empty like "{,1}". Return RE_DUP_MAX + 1 if the number field is too large. Return -2 if an error occurred. */ static Idx fetch_number (re_string_t *input, re_token_t *token, reg_syntax_t syntax) { Idx num = -1; unsigned char c; while (1) { fetch_token (token, input, syntax); c = token->opr.c; if (BE (token->type == END_OF_RE, 0)) return -2; if (token->type == OP_CLOSE_DUP_NUM || c == ',') break; num = ((token->type != CHARACTER || c < '0' || '9' < c || num == -2) ? -2 : num == -1 ? c - '0' : MIN (RE_DUP_MAX + 1, num * 10 + c - '0')); } return num; } #ifdef RE_ENABLE_I18N static void free_charset (re_charset_t *cset) { re_free (cset->mbchars); # ifdef _LIBC re_free (cset->coll_syms); re_free (cset->equiv_classes); re_free (cset->range_starts); re_free (cset->range_ends); # endif re_free (cset->char_classes); re_free (cset); } #endif /* RE_ENABLE_I18N */ /* Functions for binary tree operation. */ /* Create a tree node. */ static bin_tree_t * create_tree (re_dfa_t *dfa, bin_tree_t *left, bin_tree_t *right, re_token_type_t type) { re_token_t t; #if defined GCC_LINT || defined lint memset (&t, 0, sizeof t); #endif t.type = type; return create_token_tree (dfa, left, right, &t); } static bin_tree_t * create_token_tree (re_dfa_t *dfa, bin_tree_t *left, bin_tree_t *right, const re_token_t *token) { bin_tree_t *tree; if (BE (dfa->str_tree_storage_idx == BIN_TREE_STORAGE_SIZE, 0)) { bin_tree_storage_t *storage = re_malloc (bin_tree_storage_t, 1); if (storage == NULL) return NULL; storage->next = dfa->str_tree_storage; dfa->str_tree_storage = storage; dfa->str_tree_storage_idx = 0; } tree = &dfa->str_tree_storage->data[dfa->str_tree_storage_idx++]; tree->parent = NULL; tree->left = left; tree->right = right; tree->token = *token; tree->token.duplicated = 0; tree->token.opt_subexp = 0; tree->first = NULL; tree->next = NULL; tree->node_idx = -1; if (left != NULL) left->parent = tree; if (right != NULL) right->parent = tree; return tree; } /* Mark the tree SRC as an optional subexpression. To be called from preorder or postorder. */ static reg_errcode_t mark_opt_subexp (void *extra, bin_tree_t *node) { Idx idx = (uintptr_t) extra; if (node->token.type == SUBEXP && node->token.opr.idx == idx) node->token.opt_subexp = 1; return REG_NOERROR; } /* Free the allocated memory inside NODE. */ static void free_token (re_token_t *node) { #ifdef RE_ENABLE_I18N if (node->type == COMPLEX_BRACKET && node->duplicated == 0) free_charset (node->opr.mbcset); else #endif /* RE_ENABLE_I18N */ if (node->type == SIMPLE_BRACKET && node->duplicated == 0) re_free (node->opr.sbcset); } /* Worker function for tree walking. Free the allocated memory inside NODE and its children. */ static reg_errcode_t free_tree (void *extra, bin_tree_t *node) { free_token (&node->token); return REG_NOERROR; } /* Duplicate the node SRC, and return new node. This is a preorder visit similar to the one implemented by the generic visitor, but we need more infrastructure to maintain two parallel trees --- so, it's easier to duplicate. */ static bin_tree_t * duplicate_tree (const bin_tree_t *root, re_dfa_t *dfa) { const bin_tree_t *node; bin_tree_t *dup_root; bin_tree_t **p_new = &dup_root, *dup_node = root->parent; for (node = root; ; ) { /* Create a new tree and link it back to the current parent. */ *p_new = create_token_tree (dfa, NULL, NULL, &node->token); if (*p_new == NULL) return NULL; (*p_new)->parent = dup_node; (*p_new)->token.duplicated = 1; dup_node = *p_new; /* Go to the left node, or up and to the right. */ if (node->left) { node = node->left; p_new = &dup_node->left; } else { const bin_tree_t *prev = NULL; while (node->right == prev || node->right == NULL) { prev = node; node = node->parent; dup_node = dup_node->parent; if (!node) return dup_root; } node = node->right; p_new = &dup_node->right; } } } gnuastro-0.2.33-8a3b/bootstrapped/lib/rawmemchr.c0000644000175000017500000001220113004436754016524 00000000000000/* Searching in a string. Copyright (C) 2008-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include /* Find the first occurrence of C in S. */ void * rawmemchr (const void *s, int c_in) { /* On 32-bit hardware, choosing longword to be a 32-bit unsigned long instead of a 64-bit uintmax_t tends to give better performance. On 64-bit hardware, unsigned long is generally 64 bits already. Change this typedef to experiment with performance. */ typedef unsigned long int longword; const unsigned char *char_ptr; const longword *longword_ptr; longword repeated_one; longword repeated_c; unsigned char c; c = (unsigned char) c_in; /* Handle the first few bytes by reading one byte at a time. Do this until CHAR_PTR is aligned on a longword boundary. */ for (char_ptr = (const unsigned char *) s; (size_t) char_ptr % sizeof (longword) != 0; ++char_ptr) if (*char_ptr == c) return (void *) char_ptr; longword_ptr = (const longword *) char_ptr; /* All these elucidatory comments refer to 4-byte longwords, but the theory applies equally well to any size longwords. */ /* Compute auxiliary longword values: repeated_one is a value which has a 1 in every byte. repeated_c has c in every byte. */ repeated_one = 0x01010101; repeated_c = c | (c << 8); repeated_c |= repeated_c << 16; if (0xffffffffU < (longword) -1) { repeated_one |= repeated_one << 31 << 1; repeated_c |= repeated_c << 31 << 1; if (8 < sizeof (longword)) { size_t i; for (i = 64; i < sizeof (longword) * 8; i *= 2) { repeated_one |= repeated_one << i; repeated_c |= repeated_c << i; } } } /* Instead of the traditional loop which tests each byte, we will test a longword at a time. The tricky part is testing if *any of the four* bytes in the longword in question are equal to NUL or c. We first use an xor with repeated_c. This reduces the task to testing whether *any of the four* bytes in longword1 is zero. We compute tmp = ((longword1 - repeated_one) & ~longword1) & (repeated_one << 7). That is, we perform the following operations: 1. Subtract repeated_one. 2. & ~longword1. 3. & a mask consisting of 0x80 in every byte. Consider what happens in each byte: - If a byte of longword1 is zero, step 1 and 2 transform it into 0xff, and step 3 transforms it into 0x80. A carry can also be propagated to more significant bytes. - If a byte of longword1 is nonzero, let its lowest 1 bit be at position k (0 <= k <= 7); so the lowest k bits are 0. After step 1, the byte ends in a single bit of value 0 and k bits of value 1. After step 2, the result is just k bits of value 1: 2^k - 1. After step 3, the result is 0. And no carry is produced. So, if longword1 has only non-zero bytes, tmp is zero. Whereas if longword1 has a zero byte, call j the position of the least significant zero byte. Then the result has a zero at positions 0, ..., j-1 and a 0x80 at position j. We cannot predict the result at the more significant bytes (positions j+1..3), but it does not matter since we already have a non-zero bit at position 8*j+7. The test whether any byte in longword1 is zero is equivalent to testing whether tmp is nonzero. This test can read beyond the end of a string, depending on where C_IN is encountered. However, this is considered safe since the initialization phase ensured that the read will be aligned, therefore, the read will not cross page boundaries and will not cause a fault. */ while (1) { longword longword1 = *longword_ptr ^ repeated_c; if ((((longword1 - repeated_one) & ~longword1) & (repeated_one << 7)) != 0) break; longword_ptr++; } char_ptr = (const unsigned char *) longword_ptr; /* At this point, we know that one of the sizeof (longword) bytes starting at char_ptr is == c. On little-endian machines, we could determine the first such byte without any further memory accesses, just by looking at the tmp result from the last loop iteration. But this does not work on big-endian machines. Choose code that works in both cases. */ char_ptr = (unsigned char *) longword_ptr; while (*char_ptr != c) char_ptr++; return (void *) char_ptr; } gnuastro-0.2.33-8a3b/bootstrapped/lib/nl_langinfo.c0000644000175000017500000002201713004436754017033 00000000000000/* nl_langinfo() replacement: query locale dependent information. Copyright (C) 2007-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # define WIN32_LEAN_AND_MEAN /* avoid including junk */ # include # include #endif /* Return the codeset of the current locale, if this is easily deducible. Otherwise, return "". */ static char * ctype_codeset (void) { static char buf[2 + 10 + 1]; char const *locale = setlocale (LC_CTYPE, NULL); char *codeset = buf; size_t codesetlen; codeset[0] = '\0'; if (locale && locale[0]) { /* If the locale name contains an encoding after the dot, return it. */ char *dot = strchr (locale, '.'); if (dot) { /* Look for the possible @... trailer and remove it, if any. */ char *codeset_start = dot + 1; char const *modifier = strchr (codeset_start, '@'); if (! modifier) codeset = codeset_start; else { codesetlen = modifier - codeset_start; if (codesetlen < sizeof buf) { codeset = memcpy (buf, codeset_start, codesetlen); codeset[codesetlen] = '\0'; } } } } #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* If setlocale is successful, it returns the number of the codepage, as a string. Otherwise, fall back on Windows API GetACP, which returns the locale's codepage as a number (although this doesn't change according to what the 'setlocale' call specified). Either way, prepend "CP" to make it a valid codeset name. */ codesetlen = strlen (codeset); if (0 < codesetlen && codesetlen < sizeof buf - 2) memmove (buf + 2, codeset, codesetlen + 1); else sprintf (buf + 2, "%u", GetACP ()); codeset = memcpy (buf, "CP", 2); #endif return codeset; } #if REPLACE_NL_LANGINFO /* Override nl_langinfo with support for added nl_item values. */ # undef nl_langinfo char * rpl_nl_langinfo (nl_item item) { switch (item) { # if GNULIB_defined_CODESET case CODESET: return ctype_codeset (); # endif # if GNULIB_defined_T_FMT_AMPM case T_FMT_AMPM: return (char *) "%I:%M:%S %p"; # endif # if GNULIB_defined_ERA case ERA: /* The format is not standardized. In glibc it is a sequence of strings of the form "direction:offset:start_date:end_date:era_name:era_format" with an empty string at the end. */ return (char *) ""; case ERA_D_FMT: /* The %Ex conversion in strftime behaves like %x if the locale does not have an alternative time format. */ item = D_FMT; break; case ERA_D_T_FMT: /* The %Ec conversion in strftime behaves like %c if the locale does not have an alternative time format. */ item = D_T_FMT; break; case ERA_T_FMT: /* The %EX conversion in strftime behaves like %X if the locale does not have an alternative time format. */ item = T_FMT; break; case ALT_DIGITS: /* The format is not standardized. In glibc it is a sequence of 10 strings, appended in memory. */ return (char *) "\0\0\0\0\0\0\0\0\0\0"; # endif # if GNULIB_defined_YESEXPR || !FUNC_NL_LANGINFO_YESEXPR_WORKS case YESEXPR: return (char *) "^[yY]"; case NOEXPR: return (char *) "^[nN]"; # endif default: break; } return nl_langinfo (item); } #else /* Provide nl_langinfo from scratch, either for native MS-Windows, or for old Unix platforms without locales, such as Linux libc5 or BeOS. */ # include char * nl_langinfo (nl_item item) { static char nlbuf[100]; struct tm tmm = { 0 }; switch (item) { /* nl_langinfo items of the LC_CTYPE category */ case CODESET: { char *codeset = ctype_codeset (); if (*codeset) return codeset; } # ifdef __BEOS__ return (char *) "UTF-8"; # else return (char *) "ISO-8859-1"; # endif /* nl_langinfo items of the LC_NUMERIC category */ case RADIXCHAR: return localeconv () ->decimal_point; case THOUSEP: return localeconv () ->thousands_sep; case GROUPING: return localeconv () ->grouping; /* nl_langinfo items of the LC_TIME category. TODO: Really use the locale. */ case D_T_FMT: case ERA_D_T_FMT: return (char *) "%a %b %e %H:%M:%S %Y"; case D_FMT: case ERA_D_FMT: return (char *) "%m/%d/%y"; case T_FMT: case ERA_T_FMT: return (char *) "%H:%M:%S"; case T_FMT_AMPM: return (char *) "%I:%M:%S %p"; case AM_STR: if (!strftime (nlbuf, sizeof nlbuf, "%p", &tmm)) return (char *) "AM"; return nlbuf; case PM_STR: tmm.tm_hour = 12; if (!strftime (nlbuf, sizeof nlbuf, "%p", &tmm)) return (char *) "PM"; return nlbuf; case DAY_1: case DAY_2: case DAY_3: case DAY_4: case DAY_5: case DAY_6: case DAY_7: { static char const days[][sizeof "Wednesday"] = { "Sunday", "Monday", "Tuesday", "Wednesday", "Thursday", "Friday", "Saturday" }; tmm.tm_wday = item - DAY_1; if (!strftime (nlbuf, sizeof nlbuf, "%A", &tmm)) return (char *) days[item - DAY_1]; return nlbuf; } case ABDAY_1: case ABDAY_2: case ABDAY_3: case ABDAY_4: case ABDAY_5: case ABDAY_6: case ABDAY_7: { static char const abdays[][sizeof "Sun"] = { "Sun", "Mon", "Tue", "Wed", "Thu", "Fri", "Sat" }; tmm.tm_wday = item - ABDAY_1; if (!strftime (nlbuf, sizeof nlbuf, "%a", &tmm)) return (char *) abdays[item - ABDAY_1]; return nlbuf; } case MON_1: case MON_2: case MON_3: case MON_4: case MON_5: case MON_6: case MON_7: case MON_8: case MON_9: case MON_10: case MON_11: case MON_12: { static char const months[][sizeof "September"] = { "January", "February", "March", "April", "May", "June", "July", "September", "October", "November", "December" }; tmm.tm_mon = item - MON_1; if (!strftime (nlbuf, sizeof nlbuf, "%B", &tmm)) return (char *) months[item - MON_1]; return nlbuf; } case ABMON_1: case ABMON_2: case ABMON_3: case ABMON_4: case ABMON_5: case ABMON_6: case ABMON_7: case ABMON_8: case ABMON_9: case ABMON_10: case ABMON_11: case ABMON_12: { static char const abmonths[][sizeof "Jan"] = { "Jan", "Feb", "Mar", "Apr", "May", "Jun", "Jul", "Sep", "Oct", "Nov", "Dec" }; tmm.tm_mon = item - ABMON_1; if (!strftime (nlbuf, sizeof nlbuf, "%b", &tmm)) return (char *) abmonths[item - ABMON_1]; return nlbuf; } case ERA: return (char *) ""; case ALT_DIGITS: return (char *) "\0\0\0\0\0\0\0\0\0\0"; /* nl_langinfo items of the LC_MONETARY category. */ case CRNCYSTR: return localeconv () ->currency_symbol; case INT_CURR_SYMBOL: return localeconv () ->int_curr_symbol; case MON_DECIMAL_POINT: return localeconv () ->mon_decimal_point; case MON_THOUSANDS_SEP: return localeconv () ->mon_thousands_sep; case MON_GROUPING: return localeconv () ->mon_grouping; case POSITIVE_SIGN: return localeconv () ->positive_sign; case NEGATIVE_SIGN: return localeconv () ->negative_sign; case FRAC_DIGITS: return & localeconv () ->frac_digits; case INT_FRAC_DIGITS: return & localeconv () ->int_frac_digits; case P_CS_PRECEDES: return & localeconv () ->p_cs_precedes; case N_CS_PRECEDES: return & localeconv () ->n_cs_precedes; case P_SEP_BY_SPACE: return & localeconv () ->p_sep_by_space; case N_SEP_BY_SPACE: return & localeconv () ->n_sep_by_space; case P_SIGN_POSN: return & localeconv () ->p_sign_posn; case N_SIGN_POSN: return & localeconv () ->n_sign_posn; /* nl_langinfo items of the LC_MESSAGES category TODO: Really use the locale. */ case YESEXPR: return (char *) "^[yY]"; case NOEXPR: return (char *) "^[nN]"; default: return (char *) ""; } } #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/msvc-nothrow.c0000644000175000017500000000243413004436754017214 00000000000000/* Wrappers that don't throw invalid parameter notifications with MSVC runtime libraries. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include "msvc-nothrow.h" /* Get declarations of the native Windows API functions. */ #define WIN32_LEAN_AND_MEAN #include #include "msvc-inval.h" #undef _get_osfhandle #if HAVE_MSVC_INVALID_PARAMETER_HANDLER intptr_t _gl_nothrow_get_osfhandle (int fd) { intptr_t result; TRY_MSVC_INVAL { result = _get_osfhandle (fd); } CATCH_MSVC_INVAL { result = (intptr_t) INVALID_HANDLE_VALUE; } DONE_MSVC_INVAL; return result; } #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/msvc-inval.c0000644000175000017500000000751113004436754016626 00000000000000/* Invalid parameter handler for MSVC runtime libraries. Copyright (C) 2011-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include "msvc-inval.h" #if HAVE_MSVC_INVALID_PARAMETER_HANDLER \ && !(MSVC_INVALID_PARAMETER_HANDLING == SANE_LIBRARY_HANDLING) /* Get _invalid_parameter_handler type and _set_invalid_parameter_handler declaration. */ # include # if MSVC_INVALID_PARAMETER_HANDLING == DEFAULT_HANDLING static void __cdecl gl_msvc_invalid_parameter_handler (const wchar_t *expression, const wchar_t *function, const wchar_t *file, unsigned int line, uintptr_t dummy) { } # else /* Get declarations of the native Windows API functions. */ # define WIN32_LEAN_AND_MEAN # include # if defined _MSC_VER static void __cdecl gl_msvc_invalid_parameter_handler (const wchar_t *expression, const wchar_t *function, const wchar_t *file, unsigned int line, uintptr_t dummy) { RaiseException (STATUS_GNULIB_INVALID_PARAMETER, 0, 0, NULL); } # else /* An index to thread-local storage. */ static DWORD tls_index; static int tls_initialized /* = 0 */; /* Used as a fallback only. */ static struct gl_msvc_inval_per_thread not_per_thread; struct gl_msvc_inval_per_thread * gl_msvc_inval_current (void) { if (!tls_initialized) { tls_index = TlsAlloc (); tls_initialized = 1; } if (tls_index == TLS_OUT_OF_INDEXES) /* TlsAlloc had failed. */ return ¬_per_thread; else { struct gl_msvc_inval_per_thread *pointer = (struct gl_msvc_inval_per_thread *) TlsGetValue (tls_index); if (pointer == NULL) { /* First call. Allocate a new 'struct gl_msvc_inval_per_thread'. */ pointer = (struct gl_msvc_inval_per_thread *) malloc (sizeof (struct gl_msvc_inval_per_thread)); if (pointer == NULL) /* Could not allocate memory. Use the global storage. */ pointer = ¬_per_thread; TlsSetValue (tls_index, pointer); } return pointer; } } static void __cdecl gl_msvc_invalid_parameter_handler (const wchar_t *expression, const wchar_t *function, const wchar_t *file, unsigned int line, uintptr_t dummy) { struct gl_msvc_inval_per_thread *current = gl_msvc_inval_current (); if (current->restart_valid) longjmp (current->restart, 1); else /* An invalid parameter notification from outside the gnulib code. Give the caller a chance to intervene. */ RaiseException (STATUS_GNULIB_INVALID_PARAMETER, 0, 0, NULL); } # endif # endif static int gl_msvc_inval_initialized /* = 0 */; void gl_msvc_inval_ensure_handler (void) { if (gl_msvc_inval_initialized == 0) { _set_invalid_parameter_handler (gl_msvc_invalid_parameter_handler); gl_msvc_inval_initialized = 1; } } #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/mempcpy.c0000644000175000017500000000200213004436754016207 00000000000000/* Copy memory area and return pointer after last written byte. Copyright (C) 2003, 2007, 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include /* Copy N bytes of SRC to DEST, return pointer to bytes after the last written byte. */ void * mempcpy (void *dest, const void *src, size_t n) { return (char *) memcpy (dest, src, n) + n; } gnuastro-0.2.33-8a3b/bootstrapped/lib/memchr.c0000644000175000017500000001334613004436754016025 00000000000000/* Copyright (C) 1991, 1993, 1996-1997, 1999-2000, 2003-2004, 2006, 2008-2016 Free Software Foundation, Inc. Based on strlen implementation by Torbjorn Granlund (tege@sics.se), with help from Dan Sahlin (dan@sics.se) and commentary by Jim Blandy (jimb@ai.mit.edu); adaptation to memchr suggested by Dick Karpinski (dick@cca.ucsf.edu), and implemented by Roland McGrath (roland@ai.mit.edu). NOTE: The canonical source of this file is maintained with the GNU C Library. Bugs can be reported to bug-glibc@prep.ai.mit.edu. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _LIBC # include #endif #include #include #if defined _LIBC # include #else # define reg_char char #endif #include #if HAVE_BP_SYM_H || defined _LIBC # include #else # define BP_SYM(sym) sym #endif #undef __memchr #ifdef _LIBC # undef memchr #endif #ifndef weak_alias # define __memchr memchr #endif /* Search no more than N bytes of S for C. */ void * __memchr (void const *s, int c_in, size_t n) { /* On 32-bit hardware, choosing longword to be a 32-bit unsigned long instead of a 64-bit uintmax_t tends to give better performance. On 64-bit hardware, unsigned long is generally 64 bits already. Change this typedef to experiment with performance. */ typedef unsigned long int longword; const unsigned char *char_ptr; const longword *longword_ptr; longword repeated_one; longword repeated_c; unsigned reg_char c; c = (unsigned char) c_in; /* Handle the first few bytes by reading one byte at a time. Do this until CHAR_PTR is aligned on a longword boundary. */ for (char_ptr = (const unsigned char *) s; n > 0 && (size_t) char_ptr % sizeof (longword) != 0; --n, ++char_ptr) if (*char_ptr == c) return (void *) char_ptr; longword_ptr = (const longword *) char_ptr; /* All these elucidatory comments refer to 4-byte longwords, but the theory applies equally well to any size longwords. */ /* Compute auxiliary longword values: repeated_one is a value which has a 1 in every byte. repeated_c has c in every byte. */ repeated_one = 0x01010101; repeated_c = c | (c << 8); repeated_c |= repeated_c << 16; if (0xffffffffU < (longword) -1) { repeated_one |= repeated_one << 31 << 1; repeated_c |= repeated_c << 31 << 1; if (8 < sizeof (longword)) { size_t i; for (i = 64; i < sizeof (longword) * 8; i *= 2) { repeated_one |= repeated_one << i; repeated_c |= repeated_c << i; } } } /* Instead of the traditional loop which tests each byte, we will test a longword at a time. The tricky part is testing if *any of the four* bytes in the longword in question are equal to c. We first use an xor with repeated_c. This reduces the task to testing whether *any of the four* bytes in longword1 is zero. We compute tmp = ((longword1 - repeated_one) & ~longword1) & (repeated_one << 7). That is, we perform the following operations: 1. Subtract repeated_one. 2. & ~longword1. 3. & a mask consisting of 0x80 in every byte. Consider what happens in each byte: - If a byte of longword1 is zero, step 1 and 2 transform it into 0xff, and step 3 transforms it into 0x80. A carry can also be propagated to more significant bytes. - If a byte of longword1 is nonzero, let its lowest 1 bit be at position k (0 <= k <= 7); so the lowest k bits are 0. After step 1, the byte ends in a single bit of value 0 and k bits of value 1. After step 2, the result is just k bits of value 1: 2^k - 1. After step 3, the result is 0. And no carry is produced. So, if longword1 has only non-zero bytes, tmp is zero. Whereas if longword1 has a zero byte, call j the position of the least significant zero byte. Then the result has a zero at positions 0, ..., j-1 and a 0x80 at position j. We cannot predict the result at the more significant bytes (positions j+1..3), but it does not matter since we already have a non-zero bit at position 8*j+7. So, the test whether any byte in longword1 is zero is equivalent to testing whether tmp is nonzero. */ while (n >= sizeof (longword)) { longword longword1 = *longword_ptr ^ repeated_c; if ((((longword1 - repeated_one) & ~longword1) & (repeated_one << 7)) != 0) break; longword_ptr++; n -= sizeof (longword); } char_ptr = (const unsigned char *) longword_ptr; /* At this point, we know that either n < sizeof (longword), or one of the sizeof (longword) bytes starting at char_ptr is == c. On little-endian machines, we could determine the first such byte without any further memory accesses, just by looking at the tmp result from the last loop iteration. But this does not work on big-endian machines. Choose code that works in both cases. */ for (; n > 0; --n, ++char_ptr) { if (*char_ptr == c) return (void *) char_ptr; } return NULL; } #ifdef weak_alias weak_alias (__memchr, BP_SYM (memchr)) #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/mbtowc.c0000644000175000017500000000164613004436754016045 00000000000000/* Convert multibyte character to wide character. Copyright (C) 2011-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2011. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include #include #include #include "mbtowc-impl.h" gnuastro-0.2.33-8a3b/bootstrapped/lib/mbsinit.c0000644000175000017500000000370313004436754016213 00000000000000/* Test for initial conversion state. Copyright (C) 2008-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2008. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include "verify.h" #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, 'mbstate_t' is defined as 'int'. */ int mbsinit (const mbstate_t *ps) { return ps == NULL || *ps == 0; } #else /* Platforms that lack mbsinit() also lack mbrlen(), mbrtowc(), mbsrtowcs() and wcrtomb(), wcsrtombs(). We assume that - sizeof (mbstate_t) >= 4, - only stateless encodings are supported (such as UTF-8 and EUC-JP, but not ISO-2022 variants), - for each encoding, the number of bytes for a wide character is <= 4. (This maximum is attained for UTF-8, GB18030, EUC-TW.) We define the meaning of mbstate_t as follows: - In mb -> wc direction, mbstate_t's first byte contains the number of buffered bytes (in the range 0..3), followed by up to 3 buffered bytes. - In wc -> mb direction, mbstate_t contains no information. In other words, it is always in the initial state. */ verify (sizeof (mbstate_t) >= 4); int mbsinit (const mbstate_t *ps) { const char *pstate = (const char *)ps; return pstate == NULL || pstate[0] == 0; } #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/mbrtowc.c0000644000175000017500000002523513004436754016227 00000000000000/* Convert multibyte character to wide character. Copyright (C) 1999-2002, 2005-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2008. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #if C_LOCALE_MAYBE_EILSEQ # include "hard-locale.h" # include #endif #if GNULIB_defined_mbstate_t /* Implement mbrtowc() on top of mbtowc(). */ # include # include # include "localcharset.h" # include "streq.h" # include "verify.h" verify (sizeof (mbstate_t) >= 4); static char internal_state[4]; size_t mbrtowc (wchar_t *pwc, const char *s, size_t n, mbstate_t *ps) { char *pstate = (char *)ps; if (s == NULL) { pwc = NULL; s = ""; n = 1; } if (n == 0) return (size_t)(-2); /* Here n > 0. */ if (pstate == NULL) pstate = internal_state; { size_t nstate = pstate[0]; char buf[4]; const char *p; size_t m; switch (nstate) { case 0: p = s; m = n; break; case 3: buf[2] = pstate[3]; /*FALLTHROUGH*/ case 2: buf[1] = pstate[2]; /*FALLTHROUGH*/ case 1: buf[0] = pstate[1]; p = buf; m = nstate; buf[m++] = s[0]; if (n >= 2 && m < 4) { buf[m++] = s[1]; if (n >= 3 && m < 4) buf[m++] = s[2]; } break; default: errno = EINVAL; return (size_t)(-1); } /* Here m > 0. */ # if __GLIBC__ || defined __UCLIBC__ /* Work around bug */ mbtowc (NULL, NULL, 0); # endif { int res = mbtowc (pwc, p, m); if (res >= 0) { if (pwc != NULL && ((*pwc == 0) != (res == 0))) abort (); if (nstate >= (res > 0 ? res : 1)) abort (); res -= nstate; pstate[0] = 0; return res; } /* mbtowc does not distinguish between invalid and incomplete multibyte sequences. But mbrtowc needs to make this distinction. There are two possible approaches: - Use iconv() and its return value. - Use built-in knowledge about the possible encodings. Given the low quality of implementation of iconv() on the systems that lack mbrtowc(), we use the second approach. The possible encodings are: - 8-bit encodings, - EUC-JP, EUC-KR, GB2312, EUC-TW, BIG5, GB18030, SJIS, - UTF-8. Use specialized code for each. */ if (m >= 4 || m >= MB_CUR_MAX) goto invalid; /* Here MB_CUR_MAX > 1 and 0 < m < 4. */ { const char *encoding = locale_charset (); if (STREQ_OPT (encoding, "UTF-8", 'U', 'T', 'F', '-', '8', 0, 0, 0, 0)) { /* Cf. unistr/u8-mblen.c. */ unsigned char c = (unsigned char) p[0]; if (c >= 0xc2) { if (c < 0xe0) { if (m == 1) goto incomplete; } else if (c < 0xf0) { if (m == 1) goto incomplete; if (m == 2) { unsigned char c2 = (unsigned char) p[1]; if ((c2 ^ 0x80) < 0x40 && (c >= 0xe1 || c2 >= 0xa0) && (c != 0xed || c2 < 0xa0)) goto incomplete; } } else if (c <= 0xf4) { if (m == 1) goto incomplete; else /* m == 2 || m == 3 */ { unsigned char c2 = (unsigned char) p[1]; if ((c2 ^ 0x80) < 0x40 && (c >= 0xf1 || c2 >= 0x90) && (c < 0xf4 || (c == 0xf4 && c2 < 0x90))) { if (m == 2) goto incomplete; else /* m == 3 */ { unsigned char c3 = (unsigned char) p[2]; if ((c3 ^ 0x80) < 0x40) goto incomplete; } } } } } goto invalid; } /* As a reference for this code, you can use the GNU libiconv implementation. Look for uses of the RET_TOOFEW macro. */ if (STREQ_OPT (encoding, "EUC-JP", 'E', 'U', 'C', '-', 'J', 'P', 0, 0, 0)) { if (m == 1) { unsigned char c = (unsigned char) p[0]; if ((c >= 0xa1 && c < 0xff) || c == 0x8e || c == 0x8f) goto incomplete; } if (m == 2) { unsigned char c = (unsigned char) p[0]; if (c == 0x8f) { unsigned char c2 = (unsigned char) p[1]; if (c2 >= 0xa1 && c2 < 0xff) goto incomplete; } } goto invalid; } if (STREQ_OPT (encoding, "EUC-KR", 'E', 'U', 'C', '-', 'K', 'R', 0, 0, 0) || STREQ_OPT (encoding, "GB2312", 'G', 'B', '2', '3', '1', '2', 0, 0, 0) || STREQ_OPT (encoding, "BIG5", 'B', 'I', 'G', '5', 0, 0, 0, 0, 0)) { if (m == 1) { unsigned char c = (unsigned char) p[0]; if (c >= 0xa1 && c < 0xff) goto incomplete; } goto invalid; } if (STREQ_OPT (encoding, "EUC-TW", 'E', 'U', 'C', '-', 'T', 'W', 0, 0, 0)) { if (m == 1) { unsigned char c = (unsigned char) p[0]; if ((c >= 0xa1 && c < 0xff) || c == 0x8e) goto incomplete; } else /* m == 2 || m == 3 */ { unsigned char c = (unsigned char) p[0]; if (c == 0x8e) goto incomplete; } goto invalid; } if (STREQ_OPT (encoding, "GB18030", 'G', 'B', '1', '8', '0', '3', '0', 0, 0)) { if (m == 1) { unsigned char c = (unsigned char) p[0]; if ((c >= 0x90 && c <= 0xe3) || (c >= 0xf8 && c <= 0xfe)) goto incomplete; } else /* m == 2 || m == 3 */ { unsigned char c = (unsigned char) p[0]; if (c >= 0x90 && c <= 0xe3) { unsigned char c2 = (unsigned char) p[1]; if (c2 >= 0x30 && c2 <= 0x39) { if (m == 2) goto incomplete; else /* m == 3 */ { unsigned char c3 = (unsigned char) p[2]; if (c3 >= 0x81 && c3 <= 0xfe) goto incomplete; } } } } goto invalid; } if (STREQ_OPT (encoding, "SJIS", 'S', 'J', 'I', 'S', 0, 0, 0, 0, 0)) { if (m == 1) { unsigned char c = (unsigned char) p[0]; if ((c >= 0x81 && c <= 0x9f) || (c >= 0xe0 && c <= 0xea) || (c >= 0xf0 && c <= 0xf9)) goto incomplete; } goto invalid; } /* An unknown multibyte encoding. */ goto incomplete; } incomplete: { size_t k = nstate; /* Here 0 <= k < m < 4. */ pstate[++k] = s[0]; if (k < m) { pstate[++k] = s[1]; if (k < m) pstate[++k] = s[2]; } if (k != m) abort (); } pstate[0] = m; return (size_t)(-2); invalid: errno = EILSEQ; /* The conversion state is undefined, says POSIX. */ return (size_t)(-1); } } } #else /* Override the system's mbrtowc() function. */ # undef mbrtowc size_t rpl_mbrtowc (wchar_t *pwc, const char *s, size_t n, mbstate_t *ps) { size_t ret; wchar_t wc; # if MBRTOWC_NULL_ARG2_BUG || MBRTOWC_RETVAL_BUG || MBRTOWC_EMPTY_INPUT_BUG if (s == NULL) { pwc = NULL; s = ""; n = 1; } # endif # if MBRTOWC_EMPTY_INPUT_BUG if (n == 0) return (size_t) -2; # endif if (! pwc) pwc = &wc; # if MBRTOWC_RETVAL_BUG { static mbstate_t internal_state; /* Override mbrtowc's internal state. We cannot call mbsinit() on the hidden internal state, but we can call it on our variable. */ if (ps == NULL) ps = &internal_state; if (!mbsinit (ps)) { /* Parse the rest of the multibyte character byte for byte. */ size_t count = 0; for (; n > 0; s++, n--) { ret = mbrtowc (&wc, s, 1, ps); if (ret == (size_t)(-1)) return (size_t)(-1); count++; if (ret != (size_t)(-2)) { /* The multibyte character has been completed. */ *pwc = wc; return (wc == 0 ? 0 : count); } } return (size_t)(-2); } } # endif ret = mbrtowc (pwc, s, n, ps); # if MBRTOWC_NUL_RETVAL_BUG if (ret < (size_t) -2 && !*pwc) return 0; # endif # if C_LOCALE_MAYBE_EILSEQ if ((size_t) -2 <= ret && n != 0 && ! hard_locale (LC_CTYPE)) { unsigned char uc = *s; *pwc = uc; return 1; } # endif return ret; } #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/malloc.c0000644000175000017500000000273213004436754016016 00000000000000/* malloc() function that is glibc compatible. Copyright (C) 1997-1998, 2006-2007, 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* written by Jim Meyering and Bruno Haible */ #define _GL_USE_STDLIB_ALLOC 1 #include /* Only the AC_FUNC_MALLOC macro defines 'malloc' already in config.h. */ #ifdef malloc # define NEED_MALLOC_GNU 1 # undef malloc /* Whereas the gnulib module 'malloc-gnu' defines HAVE_MALLOC_GNU. */ #elif GNULIB_MALLOC_GNU && !HAVE_MALLOC_GNU # define NEED_MALLOC_GNU 1 #endif #include #include /* Allocate an N-byte block of memory from the heap. If N is zero, allocate a 1-byte block. */ void * rpl_malloc (size_t n) { void *result; #if NEED_MALLOC_GNU if (n == 0) n = 1; #endif result = malloc (n); #if !HAVE_MALLOC_POSIX if (result == NULL) errno = ENOMEM; #endif return result; } gnuastro-0.2.33-8a3b/bootstrapped/lib/localeconv.c0000644000175000017500000000656213004436754016701 00000000000000/* Query locale dependent information for formatting numbers. Copyright (C) 2012-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #if HAVE_STRUCT_LCONV_DECIMAL_POINT /* Override for platforms where 'struct lconv' lacks the int_p_*, int_n_* members. */ struct lconv * localeconv (void) { static struct lconv result; # undef lconv # undef localeconv struct lconv *sys_result = localeconv (); result.decimal_point = sys_result->decimal_point; result.thousands_sep = sys_result->thousands_sep; result.grouping = sys_result->grouping; result.mon_decimal_point = sys_result->mon_decimal_point; result.mon_thousands_sep = sys_result->mon_thousands_sep; result.mon_grouping = sys_result->mon_grouping; result.positive_sign = sys_result->positive_sign; result.negative_sign = sys_result->negative_sign; result.currency_symbol = sys_result->currency_symbol; result.frac_digits = sys_result->frac_digits; result.p_cs_precedes = sys_result->p_cs_precedes; result.p_sign_posn = sys_result->p_sign_posn; result.p_sep_by_space = sys_result->p_sep_by_space; result.n_cs_precedes = sys_result->n_cs_precedes; result.n_sign_posn = sys_result->n_sign_posn; result.n_sep_by_space = sys_result->n_sep_by_space; result.int_curr_symbol = sys_result->int_curr_symbol; result.int_frac_digits = sys_result->int_frac_digits; result.int_p_cs_precedes = sys_result->p_cs_precedes; result.int_p_sign_posn = sys_result->p_sign_posn; result.int_p_sep_by_space = sys_result->p_sep_by_space; result.int_n_cs_precedes = sys_result->n_cs_precedes; result.int_n_sign_posn = sys_result->n_sign_posn; result.int_n_sep_by_space = sys_result->n_sep_by_space; return &result; } #else /* Override for platforms where 'struct lconv' is a dummy. */ # include struct lconv * localeconv (void) { static /*const*/ struct lconv result = { /* decimal_point */ ".", /* thousands_sep */ "", /* grouping */ "", /* mon_decimal_point */ "", /* mon_thousands_sep */ "", /* mon_grouping */ "", /* positive_sign */ "", /* negative_sign */ "", /* currency_symbol */ "", /* frac_digits */ CHAR_MAX, /* p_cs_precedes */ CHAR_MAX, /* p_sign_posn */ CHAR_MAX, /* p_sep_by_space */ CHAR_MAX, /* n_cs_precedes */ CHAR_MAX, /* n_sign_posn */ CHAR_MAX, /* n_sep_by_space */ CHAR_MAX, /* int_curr_symbol */ "", /* int_frac_digits */ CHAR_MAX, /* int_p_cs_precedes */ CHAR_MAX, /* int_p_sign_posn */ CHAR_MAX, /* int_p_sep_by_space */ CHAR_MAX, /* int_n_cs_precedes */ CHAR_MAX, /* int_n_sign_posn */ CHAR_MAX, /* int_n_sep_by_space */ CHAR_MAX }; return &result; } #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/getopt1.c0000644000175000017500000001055213004436754016131 00000000000000/* getopt_long and getopt_long_only entry points for GNU getopt. Copyright (C) 1987-1994, 1996-1998, 2004, 2006, 2009-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifdef _LIBC # include #else # include # include "getopt.h" #endif #include "getopt_int.h" #include /* This needs to come after some library #include to get __GNU_LIBRARY__ defined. */ #ifdef __GNU_LIBRARY__ #include #endif #ifndef NULL #define NULL 0 #endif int getopt_long (int argc, char *__getopt_argv_const *argv, const char *options, const struct option *long_options, int *opt_index) { return _getopt_internal (argc, (char **) argv, options, long_options, opt_index, 0, 0); } int _getopt_long_r (int argc, char **argv, const char *options, const struct option *long_options, int *opt_index, struct _getopt_data *d) { return _getopt_internal_r (argc, argv, options, long_options, opt_index, 0, d, 0); } /* Like getopt_long, but '-' as well as '--' can indicate a long option. If an option that starts with '-' (not '--') doesn't match a long option, but does match a short option, it is parsed as a short option instead. */ int getopt_long_only (int argc, char *__getopt_argv_const *argv, const char *options, const struct option *long_options, int *opt_index) { return _getopt_internal (argc, (char **) argv, options, long_options, opt_index, 1, 0); } int _getopt_long_only_r (int argc, char **argv, const char *options, const struct option *long_options, int *opt_index, struct _getopt_data *d) { return _getopt_internal_r (argc, argv, options, long_options, opt_index, 1, d, 0); } #ifdef TEST #include int main (int argc, char **argv) { int c; int digit_optind = 0; while (1) { int this_option_optind = optind ? optind : 1; int option_index = 0; static const struct option long_options[] = { {"add", 1, 0, 0}, {"append", 0, 0, 0}, {"delete", 1, 0, 0}, {"verbose", 0, 0, 0}, {"create", 0, 0, 0}, {"file", 1, 0, 0}, {0, 0, 0, 0} }; c = getopt_long (argc, argv, "abc:d:0123456789", long_options, &option_index); if (c == -1) break; switch (c) { case 0: printf ("option %s", long_options[option_index].name); if (optarg) printf (" with arg %s", optarg); printf ("\n"); break; case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': if (digit_optind != 0 && digit_optind != this_option_optind) printf ("digits occur in two different argv-elements.\n"); digit_optind = this_option_optind; printf ("option %c\n", c); break; case 'a': printf ("option a\n"); break; case 'b': printf ("option b\n"); break; case 'c': printf ("option c with value '%s'\n", optarg); break; case 'd': printf ("option d with value '%s'\n", optarg); break; case '?': break; default: printf ("?? getopt returned character code 0%o ??\n", c); } } if (optind < argc) { printf ("non-option ARGV-elements: "); while (optind < argc) printf ("%s ", argv[optind++]); printf ("\n"); } exit (0); } #endif /* TEST */ gnuastro-0.2.33-8a3b/bootstrapped/lib/getopt.c0000644000175000017500000012140613004436754016051 00000000000000/* Getopt for GNU. NOTE: getopt is part of the C library, so if you don't know what "Keep this file name-space clean" means, talk to drepper@gnu.org before changing it! Copyright (C) 1987-1996, 1998-2004, 2006, 2008-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _LIBC # include #endif #include "getopt.h" #include #include #include #include #ifdef _LIBC # include #else # include "gettext.h" # define _(msgid) gettext (msgid) #endif #if defined _LIBC && defined USE_IN_LIBIO # include #endif /* This version of 'getopt' appears to the caller like standard Unix 'getopt' but it behaves differently for the user, since it allows the user to intersperse the options with the other arguments. As 'getopt_long' works, it permutes the elements of ARGV so that, when it is done, all the options precede everything else. Thus all application programs are extended to handle flexible argument order. Using 'getopt' or setting the environment variable POSIXLY_CORRECT disables permutation. Then the behavior is completely standard. GNU application programs can use a third alternative mode in which they can distinguish the relative order of options and other arguments. */ #include "getopt_int.h" /* For communication from 'getopt' to the caller. When 'getopt' finds an option that takes an argument, the argument value is returned here. Also, when 'ordering' is RETURN_IN_ORDER, each non-option ARGV-element is returned here. */ char *optarg; /* Index in ARGV of the next element to be scanned. This is used for communication to and from the caller and for communication between successive calls to 'getopt'. On entry to 'getopt', zero means this is the first call; initialize. When 'getopt' returns -1, this is the index of the first of the non-option elements that the caller should itself scan. Otherwise, 'optind' communicates from one call to the next how much of ARGV has been scanned so far. */ /* 1003.2 says this must be 1 before any call. */ int optind = 1; /* Callers store zero here to inhibit the error message for unrecognized options. */ int opterr = 1; /* Set to an option character which was unrecognized. This must be initialized on some systems to avoid linking in the system's own getopt implementation. */ int optopt = '?'; /* Keep a global copy of all internal members of getopt_data. */ static struct _getopt_data getopt_data; #if defined HAVE_DECL_GETENV && !HAVE_DECL_GETENV extern char *getenv (); #endif #ifdef _LIBC /* Stored original parameters. XXX This is no good solution. We should rather copy the args so that we can compare them later. But we must not use malloc(3). */ extern int __libc_argc; extern char **__libc_argv; /* Bash 2.0 gives us an environment variable containing flags indicating ARGV elements that should not be considered arguments. */ # ifdef USE_NONOPTION_FLAGS /* Defined in getopt_init.c */ extern char *__getopt_nonoption_flags; # endif # ifdef USE_NONOPTION_FLAGS # define SWAP_FLAGS(ch1, ch2) \ if (d->__nonoption_flags_len > 0) \ { \ char __tmp = __getopt_nonoption_flags[ch1]; \ __getopt_nonoption_flags[ch1] = __getopt_nonoption_flags[ch2]; \ __getopt_nonoption_flags[ch2] = __tmp; \ } # else # define SWAP_FLAGS(ch1, ch2) # endif #else /* !_LIBC */ # define SWAP_FLAGS(ch1, ch2) #endif /* _LIBC */ /* Exchange two adjacent subsequences of ARGV. One subsequence is elements [first_nonopt,last_nonopt) which contains all the non-options that have been skipped so far. The other is elements [last_nonopt,optind), which contains all the options processed since those non-options were skipped. 'first_nonopt' and 'last_nonopt' are relocated so that they describe the new indices of the non-options in ARGV after they are moved. */ static void exchange (char **argv, struct _getopt_data *d) { int bottom = d->__first_nonopt; int middle = d->__last_nonopt; int top = d->optind; char *tem; /* Exchange the shorter segment with the far end of the longer segment. That puts the shorter segment into the right place. It leaves the longer segment in the right place overall, but it consists of two parts that need to be swapped next. */ #if defined _LIBC && defined USE_NONOPTION_FLAGS /* First make sure the handling of the '__getopt_nonoption_flags' string can work normally. Our top argument must be in the range of the string. */ if (d->__nonoption_flags_len > 0 && top >= d->__nonoption_flags_max_len) { /* We must extend the array. The user plays games with us and presents new arguments. */ char *new_str = malloc (top + 1); if (new_str == NULL) d->__nonoption_flags_len = d->__nonoption_flags_max_len = 0; else { memset (__mempcpy (new_str, __getopt_nonoption_flags, d->__nonoption_flags_max_len), '\0', top + 1 - d->__nonoption_flags_max_len); d->__nonoption_flags_max_len = top + 1; __getopt_nonoption_flags = new_str; } } #endif while (top > middle && middle > bottom) { if (top - middle > middle - bottom) { /* Bottom segment is the short one. */ int len = middle - bottom; register int i; /* Swap it with the top part of the top segment. */ for (i = 0; i < len; i++) { tem = argv[bottom + i]; argv[bottom + i] = argv[top - (middle - bottom) + i]; argv[top - (middle - bottom) + i] = tem; SWAP_FLAGS (bottom + i, top - (middle - bottom) + i); } /* Exclude the moved bottom segment from further swapping. */ top -= len; } else { /* Top segment is the short one. */ int len = top - middle; register int i; /* Swap it with the bottom part of the bottom segment. */ for (i = 0; i < len; i++) { tem = argv[bottom + i]; argv[bottom + i] = argv[middle + i]; argv[middle + i] = tem; SWAP_FLAGS (bottom + i, middle + i); } /* Exclude the moved top segment from further swapping. */ bottom += len; } } /* Update records for the slots the non-options now occupy. */ d->__first_nonopt += (d->optind - d->__last_nonopt); d->__last_nonopt = d->optind; } /* Initialize the internal data when the first call is made. */ static const char * _getopt_initialize (int argc _GL_UNUSED, char **argv _GL_UNUSED, const char *optstring, struct _getopt_data *d, int posixly_correct) { /* Start processing options with ARGV-element 1 (since ARGV-element 0 is the program name); the sequence of previously skipped non-option ARGV-elements is empty. */ d->__first_nonopt = d->__last_nonopt = d->optind; d->__nextchar = NULL; d->__posixly_correct = posixly_correct || !!getenv ("POSIXLY_CORRECT"); /* Determine how to handle the ordering of options and nonoptions. */ if (optstring[0] == '-') { d->__ordering = RETURN_IN_ORDER; ++optstring; } else if (optstring[0] == '+') { d->__ordering = REQUIRE_ORDER; ++optstring; } else if (d->__posixly_correct) d->__ordering = REQUIRE_ORDER; else d->__ordering = PERMUTE; #if defined _LIBC && defined USE_NONOPTION_FLAGS if (!d->__posixly_correct && argc == __libc_argc && argv == __libc_argv) { if (d->__nonoption_flags_max_len == 0) { if (__getopt_nonoption_flags == NULL || __getopt_nonoption_flags[0] == '\0') d->__nonoption_flags_max_len = -1; else { const char *orig_str = __getopt_nonoption_flags; int len = d->__nonoption_flags_max_len = strlen (orig_str); if (d->__nonoption_flags_max_len < argc) d->__nonoption_flags_max_len = argc; __getopt_nonoption_flags = (char *) malloc (d->__nonoption_flags_max_len); if (__getopt_nonoption_flags == NULL) d->__nonoption_flags_max_len = -1; else memset (__mempcpy (__getopt_nonoption_flags, orig_str, len), '\0', d->__nonoption_flags_max_len - len); } } d->__nonoption_flags_len = d->__nonoption_flags_max_len; } else d->__nonoption_flags_len = 0; #endif return optstring; } /* Scan elements of ARGV (whose length is ARGC) for option characters given in OPTSTRING. If an element of ARGV starts with '-', and is not exactly "-" or "--", then it is an option element. The characters of this element (aside from the initial '-') are option characters. If 'getopt' is called repeatedly, it returns successively each of the option characters from each of the option elements. If 'getopt' finds another option character, it returns that character, updating 'optind' and 'nextchar' so that the next call to 'getopt' can resume the scan with the following option character or ARGV-element. If there are no more option characters, 'getopt' returns -1. Then 'optind' is the index in ARGV of the first ARGV-element that is not an option. (The ARGV-elements have been permuted so that those that are not options now come last.) OPTSTRING is a string containing the legitimate option characters. If an option character is seen that is not listed in OPTSTRING, return '?' after printing an error message. If you set 'opterr' to zero, the error message is suppressed but we still return '?'. If a char in OPTSTRING is followed by a colon, that means it wants an arg, so the following text in the same ARGV-element, or the text of the following ARGV-element, is returned in 'optarg'. Two colons mean an option that wants an optional arg; if there is text in the current ARGV-element, it is returned in 'optarg', otherwise 'optarg' is set to zero. If OPTSTRING starts with '-' or '+', it requests different methods of handling the non-option ARGV-elements. See the comments about RETURN_IN_ORDER and REQUIRE_ORDER, above. Long-named options begin with '--' instead of '-'. Their names may be abbreviated as long as the abbreviation is unique or is an exact match for some defined option. If they have an argument, it follows the option name in the same ARGV-element, separated from the option name by a '=', or else the in next ARGV-element. When 'getopt' finds a long-named option, it returns 0 if that option's 'flag' field is nonzero, the value of the option's 'val' field if the 'flag' field is zero. The elements of ARGV aren't really const, because we permute them. But we pretend they're const in the prototype to be compatible with other systems. LONGOPTS is a vector of 'struct option' terminated by an element containing a name which is zero. LONGIND returns the index in LONGOPT of the long-named option found. It is only valid when a long-named option has been found by the most recent call. If LONG_ONLY is nonzero, '-' as well as '--' can introduce long-named options. */ int _getopt_internal_r (int argc, char **argv, const char *optstring, const struct option *longopts, int *longind, int long_only, struct _getopt_data *d, int posixly_correct) { int print_errors = d->opterr; if (argc < 1) return -1; d->optarg = NULL; if (d->optind == 0 || !d->__initialized) { if (d->optind == 0) d->optind = 1; /* Don't scan ARGV[0], the program name. */ optstring = _getopt_initialize (argc, argv, optstring, d, posixly_correct); d->__initialized = 1; } else if (optstring[0] == '-' || optstring[0] == '+') optstring++; if (optstring[0] == ':') print_errors = 0; /* Test whether ARGV[optind] points to a non-option argument. Either it does not have option syntax, or there is an environment flag from the shell indicating it is not an option. The later information is only used when the used in the GNU libc. */ #if defined _LIBC && defined USE_NONOPTION_FLAGS # define NONOPTION_P (argv[d->optind][0] != '-' || argv[d->optind][1] == '\0' \ || (d->optind < d->__nonoption_flags_len \ && __getopt_nonoption_flags[d->optind] == '1')) #else # define NONOPTION_P (argv[d->optind][0] != '-' || argv[d->optind][1] == '\0') #endif if (d->__nextchar == NULL || *d->__nextchar == '\0') { /* Advance to the next ARGV-element. */ /* Give FIRST_NONOPT & LAST_NONOPT rational values if OPTIND has been moved back by the user (who may also have changed the arguments). */ if (d->__last_nonopt > d->optind) d->__last_nonopt = d->optind; if (d->__first_nonopt > d->optind) d->__first_nonopt = d->optind; if (d->__ordering == PERMUTE) { /* If we have just processed some options following some non-options, exchange them so that the options come first. */ if (d->__first_nonopt != d->__last_nonopt && d->__last_nonopt != d->optind) exchange ((char **) argv, d); else if (d->__last_nonopt != d->optind) d->__first_nonopt = d->optind; /* Skip any additional non-options and extend the range of non-options previously skipped. */ while (d->optind < argc && NONOPTION_P) d->optind++; d->__last_nonopt = d->optind; } /* The special ARGV-element '--' means premature end of options. Skip it like a null option, then exchange with previous non-options as if it were an option, then skip everything else like a non-option. */ if (d->optind != argc && !strcmp (argv[d->optind], "--")) { d->optind++; if (d->__first_nonopt != d->__last_nonopt && d->__last_nonopt != d->optind) exchange ((char **) argv, d); else if (d->__first_nonopt == d->__last_nonopt) d->__first_nonopt = d->optind; d->__last_nonopt = argc; d->optind = argc; } /* If we have done all the ARGV-elements, stop the scan and back over any non-options that we skipped and permuted. */ if (d->optind == argc) { /* Set the next-arg-index to point at the non-options that we previously skipped, so the caller will digest them. */ if (d->__first_nonopt != d->__last_nonopt) d->optind = d->__first_nonopt; return -1; } /* If we have come to a non-option and did not permute it, either stop the scan or describe it to the caller and pass it by. */ if (NONOPTION_P) { if (d->__ordering == REQUIRE_ORDER) return -1; d->optarg = argv[d->optind++]; return 1; } /* We have found another option-ARGV-element. Skip the initial punctuation. */ d->__nextchar = (argv[d->optind] + 1 + (longopts != NULL && argv[d->optind][1] == '-')); } /* Decode the current option-ARGV-element. */ /* Check whether the ARGV-element is a long option. If long_only and the ARGV-element has the form "-f", where f is a valid short option, don't consider it an abbreviated form of a long option that starts with f. Otherwise there would be no way to give the -f short option. On the other hand, if there's a long option "fubar" and the ARGV-element is "-fu", do consider that an abbreviation of the long option, just like "--fu", and not "-f" with arg "u". This distinction seems to be the most useful approach. */ if (longopts != NULL && (argv[d->optind][1] == '-' || (long_only && (argv[d->optind][2] || !strchr (optstring, argv[d->optind][1]))))) { char *nameend; unsigned int namelen; const struct option *p; const struct option *pfound = NULL; struct option_list { const struct option *p; struct option_list *next; } *ambig_list = NULL; #ifdef _LIBC /* malloc() not used for _LIBC to simplify failure messages. */ # define free_option_list(l) #else # define free_option_list(l) \ while (l != NULL) \ { \ struct option_list *pn = l->next; \ free (l); \ l = pn; \ } #endif int exact = 0; int ambig = 0; int indfound = -1; int option_index; for (nameend = d->__nextchar; *nameend && *nameend != '='; nameend++) /* Do nothing. */ ; namelen = nameend - d->__nextchar; /* Test all long options for either exact match or abbreviated matches. */ for (p = longopts, option_index = 0; p->name; p++, option_index++) if (!strncmp (p->name, d->__nextchar, namelen)) { if (namelen == (unsigned int) strlen (p->name)) { /* Exact match found. */ pfound = p; indfound = option_index; exact = 1; break; } else if (pfound == NULL) { /* First nonexact match found. */ pfound = p; indfound = option_index; } else if (ambig) ; /* Taking simpler path to handling ambiguities. */ else if (long_only || pfound->has_arg != p->has_arg || pfound->flag != p->flag || pfound->val != p->val) { /* Second or later nonexact match found. */ #ifdef _LIBC struct option_list *newp = alloca (sizeof (*newp)); #else struct option_list *newp = malloc (sizeof (*newp)); if (newp == NULL) { free_option_list (ambig_list); ambig_list = NULL; ambig = 1; /* Use simpler fallback message. */ } else #endif { newp->p = p; newp->next = ambig_list; ambig_list = newp; } } } if ((ambig || ambig_list) && !exact) { if (print_errors && ambig_list) { struct option_list first; first.p = pfound; first.next = ambig_list; ambig_list = &first; #if defined _LIBC && defined USE_IN_LIBIO char *buf = NULL; size_t buflen = 0; FILE *fp = open_memstream (&buf, &buflen); if (fp != NULL) { fprintf (fp, _("%s: option '%s' is ambiguous; possibilities:"), argv[0], argv[d->optind]); do { fprintf (fp, " '--%s'", ambig_list->p->name); ambig_list = ambig_list->next; } while (ambig_list != NULL); fputc_unlocked ('\n', fp); if (__builtin_expect (fclose (fp) != EOF, 1)) { _IO_flockfile (stderr); int old_flags2 = ((_IO_FILE *) stderr)->_flags2; ((_IO_FILE *) stderr)->_flags2 |= _IO_FLAGS2_NOTCANCEL; __fxprintf (NULL, "%s", buf); ((_IO_FILE *) stderr)->_flags2 = old_flags2; _IO_funlockfile (stderr); free (buf); } } #else fprintf (stderr, _("%s: option '%s' is ambiguous; possibilities:"), argv[0], argv[d->optind]); do { fprintf (stderr, " '--%s'", ambig_list->p->name); ambig_list = ambig_list->next; } while (ambig_list != NULL); fputc ('\n', stderr); #endif } else if (print_errors && ambig) { fprintf (stderr, _("%s: option '%s' is ambiguous\n"), argv[0], argv[d->optind]); } d->__nextchar += strlen (d->__nextchar); d->optind++; d->optopt = 0; free_option_list (ambig_list); return '?'; } free_option_list (ambig_list); if (pfound != NULL) { option_index = indfound; d->optind++; if (*nameend) { /* Don't test has_arg with >, because some C compilers don't allow it to be used on enums. */ if (pfound->has_arg) d->optarg = nameend + 1; else { if (print_errors) { #if defined _LIBC && defined USE_IN_LIBIO char *buf; int n; #endif if (argv[d->optind - 1][1] == '-') { /* --option */ #if defined _LIBC && defined USE_IN_LIBIO n = __asprintf (&buf, _("\ %s: option '--%s' doesn't allow an argument\n"), argv[0], pfound->name); #else fprintf (stderr, _("\ %s: option '--%s' doesn't allow an argument\n"), argv[0], pfound->name); #endif } else { /* +option or -option */ #if defined _LIBC && defined USE_IN_LIBIO n = __asprintf (&buf, _("\ %s: option '%c%s' doesn't allow an argument\n"), argv[0], argv[d->optind - 1][0], pfound->name); #else fprintf (stderr, _("\ %s: option '%c%s' doesn't allow an argument\n"), argv[0], argv[d->optind - 1][0], pfound->name); #endif } #if defined _LIBC && defined USE_IN_LIBIO if (n >= 0) { _IO_flockfile (stderr); int old_flags2 = ((_IO_FILE *) stderr)->_flags2; ((_IO_FILE *) stderr)->_flags2 |= _IO_FLAGS2_NOTCANCEL; __fxprintf (NULL, "%s", buf); ((_IO_FILE *) stderr)->_flags2 = old_flags2; _IO_funlockfile (stderr); free (buf); } #endif } d->__nextchar += strlen (d->__nextchar); d->optopt = pfound->val; return '?'; } } else if (pfound->has_arg == 1) { if (d->optind < argc) d->optarg = argv[d->optind++]; else { if (print_errors) { #if defined _LIBC && defined USE_IN_LIBIO char *buf; if (__asprintf (&buf, _("\ %s: option '--%s' requires an argument\n"), argv[0], pfound->name) >= 0) { _IO_flockfile (stderr); int old_flags2 = ((_IO_FILE *) stderr)->_flags2; ((_IO_FILE *) stderr)->_flags2 |= _IO_FLAGS2_NOTCANCEL; __fxprintf (NULL, "%s", buf); ((_IO_FILE *) stderr)->_flags2 = old_flags2; _IO_funlockfile (stderr); free (buf); } #else fprintf (stderr, _("%s: option '--%s' requires an argument\n"), argv[0], pfound->name); #endif } d->__nextchar += strlen (d->__nextchar); d->optopt = pfound->val; return optstring[0] == ':' ? ':' : '?'; } } d->__nextchar += strlen (d->__nextchar); if (longind != NULL) *longind = option_index; if (pfound->flag) { *(pfound->flag) = pfound->val; return 0; } return pfound->val; } /* Can't find it as a long option. If this is not getopt_long_only, or the option starts with '--' or is not a valid short option, then it's an error. Otherwise interpret it as a short option. */ if (!long_only || argv[d->optind][1] == '-' || strchr (optstring, *d->__nextchar) == NULL) { if (print_errors) { #if defined _LIBC && defined USE_IN_LIBIO char *buf; int n; #endif if (argv[d->optind][1] == '-') { /* --option */ #if defined _LIBC && defined USE_IN_LIBIO n = __asprintf (&buf, _("%s: unrecognized option '--%s'\n"), argv[0], d->__nextchar); #else fprintf (stderr, _("%s: unrecognized option '--%s'\n"), argv[0], d->__nextchar); #endif } else { /* +option or -option */ #if defined _LIBC && defined USE_IN_LIBIO n = __asprintf (&buf, _("%s: unrecognized option '%c%s'\n"), argv[0], argv[d->optind][0], d->__nextchar); #else fprintf (stderr, _("%s: unrecognized option '%c%s'\n"), argv[0], argv[d->optind][0], d->__nextchar); #endif } #if defined _LIBC && defined USE_IN_LIBIO if (n >= 0) { _IO_flockfile (stderr); int old_flags2 = ((_IO_FILE *) stderr)->_flags2; ((_IO_FILE *) stderr)->_flags2 |= _IO_FLAGS2_NOTCANCEL; __fxprintf (NULL, "%s", buf); ((_IO_FILE *) stderr)->_flags2 = old_flags2; _IO_funlockfile (stderr); free (buf); } #endif } d->__nextchar = (char *) ""; d->optind++; d->optopt = 0; return '?'; } } /* Look at and handle the next short option-character. */ { char c = *d->__nextchar++; const char *temp = strchr (optstring, c); /* Increment 'optind' when we start to process its last character. */ if (*d->__nextchar == '\0') ++d->optind; if (temp == NULL || c == ':' || c == ';') { if (print_errors) { #if defined _LIBC && defined USE_IN_LIBIO char *buf; int n; #endif #if defined _LIBC && defined USE_IN_LIBIO n = __asprintf (&buf, _("%s: invalid option -- '%c'\n"), argv[0], c); #else fprintf (stderr, _("%s: invalid option -- '%c'\n"), argv[0], c); #endif #if defined _LIBC && defined USE_IN_LIBIO if (n >= 0) { _IO_flockfile (stderr); int old_flags2 = ((_IO_FILE *) stderr)->_flags2; ((_IO_FILE *) stderr)->_flags2 |= _IO_FLAGS2_NOTCANCEL; __fxprintf (NULL, "%s", buf); ((_IO_FILE *) stderr)->_flags2 = old_flags2; _IO_funlockfile (stderr); free (buf); } #endif } d->optopt = c; return '?'; } /* Convenience. Treat POSIX -W foo same as long option --foo */ if (temp[0] == 'W' && temp[1] == ';') { char *nameend; const struct option *p; const struct option *pfound = NULL; int exact = 0; int ambig = 0; int indfound = 0; int option_index; if (longopts == NULL) goto no_longs; /* This is an option that requires an argument. */ if (*d->__nextchar != '\0') { d->optarg = d->__nextchar; /* If we end this ARGV-element by taking the rest as an arg, we must advance to the next element now. */ d->optind++; } else if (d->optind == argc) { if (print_errors) { #if defined _LIBC && defined USE_IN_LIBIO char *buf; if (__asprintf (&buf, _("%s: option requires an argument -- '%c'\n"), argv[0], c) >= 0) { _IO_flockfile (stderr); int old_flags2 = ((_IO_FILE *) stderr)->_flags2; ((_IO_FILE *) stderr)->_flags2 |= _IO_FLAGS2_NOTCANCEL; __fxprintf (NULL, "%s", buf); ((_IO_FILE *) stderr)->_flags2 = old_flags2; _IO_funlockfile (stderr); free (buf); } #else fprintf (stderr, _("%s: option requires an argument -- '%c'\n"), argv[0], c); #endif } d->optopt = c; if (optstring[0] == ':') c = ':'; else c = '?'; return c; } else /* We already incremented 'd->optind' once; increment it again when taking next ARGV-elt as argument. */ d->optarg = argv[d->optind++]; /* optarg is now the argument, see if it's in the table of longopts. */ for (d->__nextchar = nameend = d->optarg; *nameend && *nameend != '='; nameend++) /* Do nothing. */ ; /* Test all long options for either exact match or abbreviated matches. */ for (p = longopts, option_index = 0; p->name; p++, option_index++) if (!strncmp (p->name, d->__nextchar, nameend - d->__nextchar)) { if ((unsigned int) (nameend - d->__nextchar) == strlen (p->name)) { /* Exact match found. */ pfound = p; indfound = option_index; exact = 1; break; } else if (pfound == NULL) { /* First nonexact match found. */ pfound = p; indfound = option_index; } else if (long_only || pfound->has_arg != p->has_arg || pfound->flag != p->flag || pfound->val != p->val) /* Second or later nonexact match found. */ ambig = 1; } if (ambig && !exact) { if (print_errors) { #if defined _LIBC && defined USE_IN_LIBIO char *buf; if (__asprintf (&buf, _("%s: option '-W %s' is ambiguous\n"), argv[0], d->optarg) >= 0) { _IO_flockfile (stderr); int old_flags2 = ((_IO_FILE *) stderr)->_flags2; ((_IO_FILE *) stderr)->_flags2 |= _IO_FLAGS2_NOTCANCEL; __fxprintf (NULL, "%s", buf); ((_IO_FILE *) stderr)->_flags2 = old_flags2; _IO_funlockfile (stderr); free (buf); } #else fprintf (stderr, _("%s: option '-W %s' is ambiguous\n"), argv[0], d->optarg); #endif } d->__nextchar += strlen (d->__nextchar); d->optind++; return '?'; } if (pfound != NULL) { option_index = indfound; if (*nameend) { /* Don't test has_arg with >, because some C compilers don't allow it to be used on enums. */ if (pfound->has_arg) d->optarg = nameend + 1; else { if (print_errors) { #if defined _LIBC && defined USE_IN_LIBIO char *buf; if (__asprintf (&buf, _("\ %s: option '-W %s' doesn't allow an argument\n"), argv[0], pfound->name) >= 0) { _IO_flockfile (stderr); int old_flags2 = ((_IO_FILE *) stderr)->_flags2; ((_IO_FILE *) stderr)->_flags2 |= _IO_FLAGS2_NOTCANCEL; __fxprintf (NULL, "%s", buf); ((_IO_FILE *) stderr)->_flags2 = old_flags2; _IO_funlockfile (stderr); free (buf); } #else fprintf (stderr, _("\ %s: option '-W %s' doesn't allow an argument\n"), argv[0], pfound->name); #endif } d->__nextchar += strlen (d->__nextchar); return '?'; } } else if (pfound->has_arg == 1) { if (d->optind < argc) d->optarg = argv[d->optind++]; else { if (print_errors) { #if defined _LIBC && defined USE_IN_LIBIO char *buf; if (__asprintf (&buf, _("\ %s: option '-W %s' requires an argument\n"), argv[0], pfound->name) >= 0) { _IO_flockfile (stderr); int old_flags2 = ((_IO_FILE *) stderr)->_flags2; ((_IO_FILE *) stderr)->_flags2 |= _IO_FLAGS2_NOTCANCEL; __fxprintf (NULL, "%s", buf); ((_IO_FILE *) stderr)->_flags2 = old_flags2; _IO_funlockfile (stderr); free (buf); } #else fprintf (stderr, _("\ %s: option '-W %s' requires an argument\n"), argv[0], pfound->name); #endif } d->__nextchar += strlen (d->__nextchar); return optstring[0] == ':' ? ':' : '?'; } } else d->optarg = NULL; d->__nextchar += strlen (d->__nextchar); if (longind != NULL) *longind = option_index; if (pfound->flag) { *(pfound->flag) = pfound->val; return 0; } return pfound->val; } no_longs: d->__nextchar = NULL; return 'W'; /* Let the application handle it. */ } if (temp[1] == ':') { if (temp[2] == ':') { /* This is an option that accepts an argument optionally. */ if (*d->__nextchar != '\0') { d->optarg = d->__nextchar; d->optind++; } else d->optarg = NULL; d->__nextchar = NULL; } else { /* This is an option that requires an argument. */ if (*d->__nextchar != '\0') { d->optarg = d->__nextchar; /* If we end this ARGV-element by taking the rest as an arg, we must advance to the next element now. */ d->optind++; } else if (d->optind == argc) { if (print_errors) { #if defined _LIBC && defined USE_IN_LIBIO char *buf; if (__asprintf (&buf, _("\ %s: option requires an argument -- '%c'\n"), argv[0], c) >= 0) { _IO_flockfile (stderr); int old_flags2 = ((_IO_FILE *) stderr)->_flags2; ((_IO_FILE *) stderr)->_flags2 |= _IO_FLAGS2_NOTCANCEL; __fxprintf (NULL, "%s", buf); ((_IO_FILE *) stderr)->_flags2 = old_flags2; _IO_funlockfile (stderr); free (buf); } #else fprintf (stderr, _("%s: option requires an argument -- '%c'\n"), argv[0], c); #endif } d->optopt = c; if (optstring[0] == ':') c = ':'; else c = '?'; } else /* We already incremented 'optind' once; increment it again when taking next ARGV-elt as argument. */ d->optarg = argv[d->optind++]; d->__nextchar = NULL; } } return c; } } int _getopt_internal (int argc, char **argv, const char *optstring, const struct option *longopts, int *longind, int long_only, int posixly_correct) { int result; getopt_data.optind = optind; getopt_data.opterr = opterr; result = _getopt_internal_r (argc, argv, optstring, longopts, longind, long_only, &getopt_data, posixly_correct); optind = getopt_data.optind; optarg = getopt_data.optarg; optopt = getopt_data.optopt; return result; } /* glibc gets a LSB-compliant getopt. Standalone applications get a POSIX-compliant getopt. */ #if _LIBC enum { POSIXLY_CORRECT = 0 }; #else enum { POSIXLY_CORRECT = 1 }; #endif int getopt (int argc, char *const *argv, const char *optstring) { return _getopt_internal (argc, (char **) argv, optstring, (const struct option *) 0, (int *) 0, 0, POSIXLY_CORRECT); } #ifdef _LIBC int __posix_getopt (int argc, char *const *argv, const char *optstring) { return _getopt_internal (argc, argv, optstring, (const struct option *) 0, (int *) 0, 0, 1); } #endif #ifdef TEST /* Compile with -DTEST to make an executable for use in testing the above definition of 'getopt'. */ int main (int argc, char **argv) { int c; int digit_optind = 0; while (1) { int this_option_optind = optind ? optind : 1; c = getopt (argc, argv, "abc:d:0123456789"); if (c == -1) break; switch (c) { case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': if (digit_optind != 0 && digit_optind != this_option_optind) printf ("digits occur in two different argv-elements.\n"); digit_optind = this_option_optind; printf ("option %c\n", c); break; case 'a': printf ("option a\n"); break; case 'b': printf ("option b\n"); break; case 'c': printf ("option c with value '%s'\n", optarg); break; case '?': break; default: printf ("?? getopt returned character code 0%o ??\n", c); } } if (optind < argc) { printf ("non-option ARGV-elements: "); while (optind < argc) printf ("%s ", argv[optind++]); printf ("\n"); } exit (0); } #endif /* TEST */ gnuastro-0.2.33-8a3b/bootstrapped/lib/itold.c0000644000175000017500000000201013004436754015647 00000000000000/* Replacement for 'int' to 'long double' conversion routine. Copyright (C) 2011-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2011. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include void _Qp_itoq (long double *result, int a) { /* Convert from 'int' to 'double', then from 'double' to 'long double'. */ *result = (double) a; } gnuastro-0.2.33-8a3b/bootstrapped/lib/float.c0000644000175000017500000000250413004436754015651 00000000000000/* Auxiliary definitions for . Copyright (C) 2011-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2011. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #if (defined _ARCH_PPC || defined _POWER) && (defined _AIX || defined __linux__) && (LDBL_MANT_DIG == 106) && defined __GNUC__ const union gl_long_double_union gl_LDBL_MAX = { { DBL_MAX, DBL_MAX / (double)134217728UL / (double)134217728UL } }; #elif defined __i386__ const union gl_long_double_union gl_LDBL_MAX = { { 0xFFFFFFFF, 0xFFFFFFFF, 32766 } }; #else /* This declaration is solely to ensure that after preprocessing this file is never empty. */ typedef int dummy; #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/error.c0000644000175000017500000002431613004436754015702 00000000000000/* Error handler for noninteractive utilities Copyright (C) 1990-1998, 2000-2007, 2009-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by David MacKenzie . */ #if !_LIBC # include #endif #include "error.h" #include #include #include #include #if !_LIBC && ENABLE_NLS # include "gettext.h" # define _(msgid) gettext (msgid) #endif #ifdef _LIBC # include # include # include # include # define mbsrtowcs __mbsrtowcs # define USE_UNLOCKED_IO 0 # define _GL_ATTRIBUTE_FORMAT_PRINTF(a, b) # define _GL_ARG_NONNULL(a) #else # include "getprogname.h" #endif #if USE_UNLOCKED_IO # include "unlocked-io.h" #endif #ifndef _ # define _(String) String #endif /* If NULL, error will flush stdout, then print on stderr the program name, a colon and a space. Otherwise, error will call this function without parameters instead. */ void (*error_print_progname) (void); /* This variable is incremented each time 'error' is called. */ unsigned int error_message_count; #ifdef _LIBC /* In the GNU C library, there is a predefined variable for this. */ # define program_name program_invocation_name # include # include # include /* In GNU libc we want do not want to use the common name 'error' directly. Instead make it a weak alias. */ extern void __error (int status, int errnum, const char *message, ...) __attribute__ ((__format__ (__printf__, 3, 4))); extern void __error_at_line (int status, int errnum, const char *file_name, unsigned int line_number, const char *message, ...) __attribute__ ((__format__ (__printf__, 5, 6))); # define error __error # define error_at_line __error_at_line # include # define fflush(s) _IO_fflush (s) # undef putc # define putc(c, fp) _IO_putc (c, fp) # include #else /* not _LIBC */ # include # include # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Get declarations of the native Windows API functions. */ # define WIN32_LEAN_AND_MEAN # include /* Get _get_osfhandle. */ # include "msvc-nothrow.h" # endif /* The gnulib override of fcntl is not needed in this file. */ # undef fcntl # if !HAVE_DECL_STRERROR_R # ifndef HAVE_DECL_STRERROR_R "this configure-time declaration test was not run" # endif # if STRERROR_R_CHAR_P char *strerror_r (); # else int strerror_r (); # endif # endif #define program_name getprogname () # if HAVE_STRERROR_R || defined strerror_r # define __strerror_r strerror_r # endif /* HAVE_STRERROR_R || defined strerror_r */ #endif /* not _LIBC */ #if !_LIBC /* Return non-zero if FD is open. */ static int is_open (int fd) { # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* On native Windows: The initial state of unassigned standard file descriptors is that they are open but point to an INVALID_HANDLE_VALUE. There is no fcntl, and the gnulib replacement fcntl does not support F_GETFL. */ return (HANDLE) _get_osfhandle (fd) != INVALID_HANDLE_VALUE; # else # ifndef F_GETFL # error Please port fcntl to your platform # endif return 0 <= fcntl (fd, F_GETFL); # endif } #endif static void flush_stdout (void) { #if !_LIBC int stdout_fd; # if GNULIB_FREOPEN_SAFER /* Use of gnulib's freopen-safer module normally ensures that fileno (stdout) == 1 whenever stdout is open. */ stdout_fd = STDOUT_FILENO; # else /* POSIX states that fileno (stdout) after fclose is unspecified. But in practice it is not a problem, because stdout is statically allocated and the fd of a FILE stream is stored as a field in its allocated memory. */ stdout_fd = fileno (stdout); # endif /* POSIX states that fflush (stdout) after fclose is unspecified; it is safe in glibc, but not on all other platforms. fflush (NULL) is always defined, but too draconian. */ if (0 <= stdout_fd && is_open (stdout_fd)) #endif fflush (stdout); } static void print_errno_message (int errnum) { char const *s; #if defined HAVE_STRERROR_R || _LIBC char errbuf[1024]; # if _LIBC || STRERROR_R_CHAR_P s = __strerror_r (errnum, errbuf, sizeof errbuf); # else if (__strerror_r (errnum, errbuf, sizeof errbuf) == 0) s = errbuf; else s = 0; # endif #else s = strerror (errnum); #endif #if !_LIBC if (! s) s = _("Unknown system error"); #endif #if _LIBC __fxprintf (NULL, ": %s", s); #else fprintf (stderr, ": %s", s); #endif } static void _GL_ATTRIBUTE_FORMAT_PRINTF (3, 0) _GL_ARG_NONNULL ((3)) error_tail (int status, int errnum, const char *message, va_list args) { #if _LIBC if (_IO_fwide (stderr, 0) > 0) { size_t len = strlen (message) + 1; wchar_t *wmessage = NULL; mbstate_t st; size_t res; const char *tmp; bool use_malloc = false; while (1) { if (__libc_use_alloca (len * sizeof (wchar_t))) wmessage = (wchar_t *) alloca (len * sizeof (wchar_t)); else { if (!use_malloc) wmessage = NULL; wchar_t *p = (wchar_t *) realloc (wmessage, len * sizeof (wchar_t)); if (p == NULL) { free (wmessage); fputws_unlocked (L"out of memory\n", stderr); return; } wmessage = p; use_malloc = true; } memset (&st, '\0', sizeof (st)); tmp = message; res = mbsrtowcs (wmessage, &tmp, len, &st); if (res != len) break; if (__builtin_expect (len >= SIZE_MAX / sizeof (wchar_t) / 2, 0)) { /* This really should not happen if everything is fine. */ res = (size_t) -1; break; } len *= 2; } if (res == (size_t) -1) { /* The string cannot be converted. */ if (use_malloc) { free (wmessage); use_malloc = false; } wmessage = (wchar_t *) L"???"; } __vfwprintf (stderr, wmessage, args); if (use_malloc) free (wmessage); } else #endif vfprintf (stderr, message, args); va_end (args); ++error_message_count; if (errnum) print_errno_message (errnum); #if _LIBC __fxprintf (NULL, "\n"); #else putc ('\n', stderr); #endif fflush (stderr); if (status) exit (status); } /* Print the program name and error message MESSAGE, which is a printf-style format string with optional args. If ERRNUM is nonzero, print its corresponding system error message. Exit with status STATUS if it is nonzero. */ void error (int status, int errnum, const char *message, ...) { va_list args; #if defined _LIBC && defined __libc_ptf_call /* We do not want this call to be cut short by a thread cancellation. Therefore disable cancellation for now. */ int state = PTHREAD_CANCEL_ENABLE; __libc_ptf_call (pthread_setcancelstate, (PTHREAD_CANCEL_DISABLE, &state), 0); #endif flush_stdout (); #ifdef _LIBC _IO_flockfile (stderr); #endif if (error_print_progname) (*error_print_progname) (); else { #if _LIBC __fxprintf (NULL, "%s: ", program_name); #else fprintf (stderr, "%s: ", program_name); #endif } va_start (args, message); error_tail (status, errnum, message, args); #ifdef _LIBC _IO_funlockfile (stderr); # ifdef __libc_ptf_call __libc_ptf_call (pthread_setcancelstate, (state, NULL), 0); # endif #endif } /* Sometimes we want to have at most one error per line. This variable controls whether this mode is selected or not. */ int error_one_per_line; void error_at_line (int status, int errnum, const char *file_name, unsigned int line_number, const char *message, ...) { va_list args; if (error_one_per_line) { static const char *old_file_name; static unsigned int old_line_number; if (old_line_number == line_number && (file_name == old_file_name || (old_file_name != NULL && file_name != NULL && strcmp (old_file_name, file_name) == 0))) /* Simply return and print nothing. */ return; old_file_name = file_name; old_line_number = line_number; } #if defined _LIBC && defined __libc_ptf_call /* We do not want this call to be cut short by a thread cancellation. Therefore disable cancellation for now. */ int state = PTHREAD_CANCEL_ENABLE; __libc_ptf_call (pthread_setcancelstate, (PTHREAD_CANCEL_DISABLE, &state), 0); #endif flush_stdout (); #ifdef _LIBC _IO_flockfile (stderr); #endif if (error_print_progname) (*error_print_progname) (); else { #if _LIBC __fxprintf (NULL, "%s:", program_name); #else fprintf (stderr, "%s:", program_name); #endif } #if _LIBC __fxprintf (NULL, file_name != NULL ? "%s:%u: " : " ", file_name, line_number); #else fprintf (stderr, file_name != NULL ? "%s:%u: " : " ", file_name, line_number); #endif va_start (args, message); error_tail (status, errnum, message, args); #ifdef _LIBC _IO_funlockfile (stderr); # ifdef __libc_ptf_call __libc_ptf_call (pthread_setcancelstate, (state, NULL), 0); # endif #endif } #ifdef _LIBC /* Make the weak alias. */ # undef error # undef error_at_line weak_alias (__error, error) weak_alias (__error_at_line, error_at_line) #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/btowc.c0000644000175000017500000000210713004436754015661 00000000000000/* Convert unibyte character to wide character. Copyright (C) 2008, 2010-2016 Free Software Foundation, Inc. Written by Bruno Haible , 2008. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include wint_t btowc (int c) { if (c != EOF) { char buf[1]; wchar_t wc; buf[0] = c; if (mbtowc (&wc, buf, 1) >= 0) return wc; } return WEOF; } gnuastro-0.2.33-8a3b/bootstrapped/lib/xsize.c0000644000175000017500000000011613004436754015703 00000000000000#include #define XSIZE_INLINE _GL_EXTERN_INLINE #include "xsize.h" gnuastro-0.2.33-8a3b/bootstrapped/lib/xsize.h0000644000175000017500000000705613004436754015722 00000000000000/* xsize.h -- Checked size_t computations. Copyright (C) 2003, 2008-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _XSIZE_H #define _XSIZE_H /* Get size_t. */ #include /* Get SIZE_MAX. */ #include #if HAVE_STDINT_H # include #endif #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef XSIZE_INLINE # define XSIZE_INLINE _GL_INLINE #endif /* The size of memory objects is often computed through expressions of type size_t. Example: void* p = malloc (header_size + n * element_size). These computations can lead to overflow. When this happens, malloc() returns a piece of memory that is way too small, and the program then crashes while attempting to fill the memory. To avoid this, the functions and macros in this file check for overflow. The convention is that SIZE_MAX represents overflow. malloc (SIZE_MAX) is not guaranteed to fail -- think of a malloc implementation that uses mmap --, it's recommended to use size_overflow_p() or size_in_bounds_p() before invoking malloc(). The example thus becomes: size_t size = xsum (header_size, xtimes (n, element_size)); void *p = (size_in_bounds_p (size) ? malloc (size) : NULL); */ /* Convert an arbitrary value >= 0 to type size_t. */ #define xcast_size_t(N) \ ((N) <= SIZE_MAX ? (size_t) (N) : SIZE_MAX) /* Sum of two sizes, with overflow check. */ XSIZE_INLINE size_t #if __GNUC__ >= 3 __attribute__ ((__pure__)) #endif xsum (size_t size1, size_t size2) { size_t sum = size1 + size2; return (sum >= size1 ? sum : SIZE_MAX); } /* Sum of three sizes, with overflow check. */ XSIZE_INLINE size_t #if __GNUC__ >= 3 __attribute__ ((__pure__)) #endif xsum3 (size_t size1, size_t size2, size_t size3) { return xsum (xsum (size1, size2), size3); } /* Sum of four sizes, with overflow check. */ XSIZE_INLINE size_t #if __GNUC__ >= 3 __attribute__ ((__pure__)) #endif xsum4 (size_t size1, size_t size2, size_t size3, size_t size4) { return xsum (xsum (xsum (size1, size2), size3), size4); } /* Maximum of two sizes, with overflow check. */ XSIZE_INLINE size_t #if __GNUC__ >= 3 __attribute__ ((__pure__)) #endif xmax (size_t size1, size_t size2) { /* No explicit check is needed here, because for any n: max (SIZE_MAX, n) == SIZE_MAX and max (n, SIZE_MAX) == SIZE_MAX. */ return (size1 >= size2 ? size1 : size2); } /* Multiplication of a count with an element size, with overflow check. The count must be >= 0 and the element size must be > 0. This is a macro, not a function, so that it works correctly even when N is of a wider type and N > SIZE_MAX. */ #define xtimes(N, ELSIZE) \ ((N) <= SIZE_MAX / (ELSIZE) ? (size_t) (N) * (ELSIZE) : SIZE_MAX) /* Check for overflow. */ #define size_overflow_p(SIZE) \ ((SIZE) == SIZE_MAX) /* Check against overflow. */ #define size_in_bounds_p(SIZE) \ ((SIZE) != SIZE_MAX) _GL_INLINE_HEADER_END #endif /* _XSIZE_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/wctype-h.c0000644000175000017500000000023313004436754016301 00000000000000/* Normally this would be wctype.c, but that name's already taken. */ #include #define _GL_WCTYPE_INLINE _GL_EXTERN_INLINE #include "wctype.h" gnuastro-0.2.33-8a3b/bootstrapped/lib/unistd.c0000644000175000017500000000014713004436754016053 00000000000000#include #define _GL_UNISTD_INLINE _GL_EXTERN_INLINE #include "unistd.h" typedef int dummy; gnuastro-0.2.33-8a3b/bootstrapped/lib/size_max.h0000644000175000017500000000221113004436754016363 00000000000000/* size_max.h -- declare SIZE_MAX through system headers Copyright (C) 2005-2006, 2009-2016 Free Software Foundation, Inc. Written by Simon Josefsson. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef GNULIB_SIZE_MAX_H #define GNULIB_SIZE_MAX_H /* Get SIZE_MAX declaration on systems like Solaris 7/8/9. */ # include /* Get SIZE_MAX declaration on systems like glibc 2. */ # if HAVE_STDINT_H # include # endif /* On systems where these include files don't define it, SIZE_MAX is defined in config.h. */ #endif /* GNULIB_SIZE_MAX_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/nproc.c0000644000175000017500000002335613004436754015675 00000000000000/* Detect the number of processors. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Glen Lenker and Bruno Haible. */ #include #include "nproc.h" #include #include #if HAVE_PTHREAD_GETAFFINITY_NP && 0 # include # include #endif #if HAVE_SCHED_GETAFFINITY_LIKE_GLIBC || HAVE_SCHED_GETAFFINITY_NP # include #endif #include #if HAVE_SYS_PSTAT_H # include #endif #if HAVE_SYS_SYSMP_H # include #endif #if HAVE_SYS_PARAM_H # include #endif #if HAVE_SYS_SYSCTL_H # include #endif #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # define WIN32_LEAN_AND_MEAN # include #endif #include "c-ctype.h" #define ARRAY_SIZE(a) (sizeof (a) / sizeof ((a)[0])) /* Return the number of processors available to the current process, based on a modern system call that returns the "affinity" between the current process and each CPU. Return 0 if unknown or if such a system call does not exist. */ static unsigned long num_processors_via_affinity_mask (void) { /* glibc >= 2.3.3 with NPTL and NetBSD 5 have pthread_getaffinity_np, but with different APIs. Also it requires linking with -lpthread. Therefore this code is not enabled. glibc >= 2.3.4 has sched_getaffinity whereas NetBSD 5 has sched_getaffinity_np. */ #if HAVE_PTHREAD_GETAFFINITY_NP && defined __GLIBC__ && 0 { cpu_set_t set; if (pthread_getaffinity_np (pthread_self (), sizeof (set), &set) == 0) { unsigned long count; # ifdef CPU_COUNT /* glibc >= 2.6 has the CPU_COUNT macro. */ count = CPU_COUNT (&set); # else size_t i; count = 0; for (i = 0; i < CPU_SETSIZE; i++) if (CPU_ISSET (i, &set)) count++; # endif if (count > 0) return count; } } #elif HAVE_PTHREAD_GETAFFINITY_NP && defined __NetBSD__ && 0 { cpuset_t *set; set = cpuset_create (); if (set != NULL) { unsigned long count = 0; if (pthread_getaffinity_np (pthread_self (), cpuset_size (set), set) == 0) { cpuid_t i; for (i = 0;; i++) { int ret = cpuset_isset (i, set); if (ret < 0) break; if (ret > 0) count++; } } cpuset_destroy (set); if (count > 0) return count; } } #elif HAVE_SCHED_GETAFFINITY_LIKE_GLIBC /* glibc >= 2.3.4 */ { cpu_set_t set; if (sched_getaffinity (0, sizeof (set), &set) == 0) { unsigned long count; # ifdef CPU_COUNT /* glibc >= 2.6 has the CPU_COUNT macro. */ count = CPU_COUNT (&set); # else size_t i; count = 0; for (i = 0; i < CPU_SETSIZE; i++) if (CPU_ISSET (i, &set)) count++; # endif if (count > 0) return count; } } #elif HAVE_SCHED_GETAFFINITY_NP /* NetBSD >= 5 */ { cpuset_t *set; set = cpuset_create (); if (set != NULL) { unsigned long count = 0; if (sched_getaffinity_np (getpid (), cpuset_size (set), set) == 0) { cpuid_t i; for (i = 0;; i++) { int ret = cpuset_isset (i, set); if (ret < 0) break; if (ret > 0) count++; } } cpuset_destroy (set); if (count > 0) return count; } } #endif #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ { /* This works on native Windows platforms. */ DWORD_PTR process_mask; DWORD_PTR system_mask; if (GetProcessAffinityMask (GetCurrentProcess (), &process_mask, &system_mask)) { DWORD_PTR mask = process_mask; unsigned long count = 0; for (; mask != 0; mask = mask >> 1) if (mask & 1) count++; if (count > 0) return count; } } #endif return 0; } unsigned long int num_processors (enum nproc_query query) { if (query == NPROC_CURRENT_OVERRIDABLE) { /* Test the environment variable OMP_NUM_THREADS, recognized also by all programs that are based on OpenMP. The OpenMP spec says that the value assigned to the environment variable "may have leading and trailing white space". */ const char *envvalue = getenv ("OMP_NUM_THREADS"); if (envvalue != NULL) { while (*envvalue != '\0' && c_isspace (*envvalue)) envvalue++; /* Convert it from decimal to 'unsigned long'. */ if (c_isdigit (*envvalue)) { char *endptr = NULL; unsigned long int value = strtoul (envvalue, &endptr, 10); if (endptr != NULL) { while (*endptr != '\0' && c_isspace (*endptr)) endptr++; if (*endptr == '\0') return (value > 0 ? value : 1); } } } query = NPROC_CURRENT; } /* Here query is one of NPROC_ALL, NPROC_CURRENT. */ /* On systems with a modern affinity mask system call, we have sysconf (_SC_NPROCESSORS_CONF) >= sysconf (_SC_NPROCESSORS_ONLN) >= num_processors_via_affinity_mask () The first number is the number of CPUs configured in the system. The second number is the number of CPUs available to the scheduler. The third number is the number of CPUs available to the current process. Note! On Linux systems with glibc, the first and second number come from the /sys and /proc file systems (see glibc/sysdeps/unix/sysv/linux/getsysstats.c). In some situations these file systems are not mounted, and the sysconf call returns 1, which does not reflect the reality. */ if (query == NPROC_CURRENT) { /* Try the modern affinity mask system call. */ { unsigned long nprocs = num_processors_via_affinity_mask (); if (nprocs > 0) return nprocs; } #if defined _SC_NPROCESSORS_ONLN { /* This works on glibc, Mac OS X 10.5, FreeBSD, AIX, OSF/1, Solaris, Cygwin, Haiku. */ long int nprocs = sysconf (_SC_NPROCESSORS_ONLN); if (nprocs > 0) return nprocs; } #endif } else /* query == NPROC_ALL */ { #if defined _SC_NPROCESSORS_CONF { /* This works on glibc, Mac OS X 10.5, FreeBSD, AIX, OSF/1, Solaris, Cygwin, Haiku. */ long int nprocs = sysconf (_SC_NPROCESSORS_CONF); # if __GLIBC__ >= 2 && defined __linux__ /* On Linux systems with glibc, this information comes from the /sys and /proc file systems (see glibc/sysdeps/unix/sysv/linux/getsysstats.c). In some situations these file systems are not mounted, and the sysconf call returns 1. But we wish to guarantee that num_processors (NPROC_ALL) >= num_processors (NPROC_CURRENT). */ if (nprocs == 1) { unsigned long nprocs_current = num_processors_via_affinity_mask (); if (nprocs_current > 0) nprocs = nprocs_current; } # endif if (nprocs > 0) return nprocs; } #endif } #if HAVE_PSTAT_GETDYNAMIC { /* This works on HP-UX. */ struct pst_dynamic psd; if (pstat_getdynamic (&psd, sizeof psd, 1, 0) >= 0) { /* The field psd_proc_cnt contains the number of active processors. In newer releases of HP-UX 11, the field psd_max_proc_cnt includes deactivated processors. */ if (query == NPROC_CURRENT) { if (psd.psd_proc_cnt > 0) return psd.psd_proc_cnt; } else { if (psd.psd_max_proc_cnt > 0) return psd.psd_max_proc_cnt; } } } #endif #if HAVE_SYSMP && defined MP_NAPROCS && defined MP_NPROCS { /* This works on IRIX. */ /* MP_NPROCS yields the number of installed processors. MP_NAPROCS yields the number of processors available to unprivileged processes. */ int nprocs = sysmp (query == NPROC_CURRENT && getpid () != 0 ? MP_NAPROCS : MP_NPROCS); if (nprocs > 0) return nprocs; } #endif /* Finally, as fallback, use the APIs that don't distinguish between NPROC_CURRENT and NPROC_ALL. */ #if HAVE_SYSCTL && defined HW_NCPU { /* This works on Mac OS X, FreeBSD, NetBSD, OpenBSD. */ int nprocs; size_t len = sizeof (nprocs); static int mib[2] = { CTL_HW, HW_NCPU }; if (sysctl (mib, ARRAY_SIZE (mib), &nprocs, &len, NULL, 0) == 0 && len == sizeof (nprocs) && 0 < nprocs) return nprocs; } #endif #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ { /* This works on native Windows platforms. */ SYSTEM_INFO system_info; GetSystemInfo (&system_info); if (0 < system_info.dwNumberOfProcessors) return system_info.dwNumberOfProcessors; } #endif return 1; } gnuastro-0.2.33-8a3b/bootstrapped/lib/math.c0000644000175000017500000000014313004436754015472 00000000000000#include #define _GL_MATH_INLINE _GL_EXTERN_INLINE #include "math.h" typedef int dummy; gnuastro-0.2.33-8a3b/bootstrapped/lib/localcharset.c0000644000175000017500000005000113004436754017203 00000000000000/* Determine a canonical name for the current locale's character encoding. Copyright (C) 2000-2006, 2008-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible . */ #include /* Specification. */ #include "localcharset.h" #include #include #include #include #include #if defined __APPLE__ && defined __MACH__ && HAVE_LANGINFO_CODESET # define DARWIN7 /* Darwin 7 or newer, i.e. Mac OS X 10.3 or newer */ #endif #if defined _WIN32 || defined __WIN32__ # define WINDOWS_NATIVE # include #endif #if defined __EMX__ /* Assume EMX program runs on OS/2, even if compiled under DOS. */ # ifndef OS2 # define OS2 # endif #endif #if !defined WINDOWS_NATIVE # include # if HAVE_LANGINFO_CODESET # include # else # if 0 /* see comment below */ # include # endif # endif # ifdef __CYGWIN__ # define WIN32_LEAN_AND_MEAN # include # endif #elif defined WINDOWS_NATIVE # define WIN32_LEAN_AND_MEAN # include #endif #if defined OS2 # define INCL_DOS # include #endif /* For MB_CUR_MAX_L */ #if defined DARWIN7 # include #endif #if ENABLE_RELOCATABLE # include "relocatable.h" #else # define relocate(pathname) (pathname) #endif /* Get LIBDIR. */ #ifndef LIBDIR # include "configmake.h" #endif /* Define O_NOFOLLOW to 0 on platforms where it does not exist. */ #ifndef O_NOFOLLOW # define O_NOFOLLOW 0 #endif #if defined _WIN32 || defined __WIN32__ || defined __CYGWIN__ || defined __EMX__ || defined __DJGPP__ /* Native Windows, Cygwin, OS/2, DOS */ # define ISSLASH(C) ((C) == '/' || (C) == '\\') #endif #ifndef DIRECTORY_SEPARATOR # define DIRECTORY_SEPARATOR '/' #endif #ifndef ISSLASH # define ISSLASH(C) ((C) == DIRECTORY_SEPARATOR) #endif #if HAVE_DECL_GETC_UNLOCKED # undef getc # define getc getc_unlocked #endif /* The following static variable is declared 'volatile' to avoid a possible multithread problem in the function get_charset_aliases. If we are running in a threaded environment, and if two threads initialize 'charset_aliases' simultaneously, both will produce the same value, and everything will be ok if the two assignments to 'charset_aliases' are atomic. But I don't know what will happen if the two assignments mix. */ #if __STDC__ != 1 # define volatile /* empty */ #endif /* Pointer to the contents of the charset.alias file, if it has already been read, else NULL. Its format is: ALIAS_1 '\0' CANONICAL_1 '\0' ... ALIAS_n '\0' CANONICAL_n '\0' '\0' */ static const char * volatile charset_aliases; /* Return a pointer to the contents of the charset.alias file. */ static const char * get_charset_aliases (void) { const char *cp; cp = charset_aliases; if (cp == NULL) { #if !(defined DARWIN7 || defined VMS || defined WINDOWS_NATIVE || defined __CYGWIN__ || defined OS2) const char *dir; const char *base = "charset.alias"; char *file_name; /* Make it possible to override the charset.alias location. This is necessary for running the testsuite before "make install". */ dir = getenv ("CHARSETALIASDIR"); if (dir == NULL || dir[0] == '\0') dir = relocate (LIBDIR); /* Concatenate dir and base into freshly allocated file_name. */ { size_t dir_len = strlen (dir); size_t base_len = strlen (base); int add_slash = (dir_len > 0 && !ISSLASH (dir[dir_len - 1])); file_name = (char *) malloc (dir_len + add_slash + base_len + 1); if (file_name != NULL) { memcpy (file_name, dir, dir_len); if (add_slash) file_name[dir_len] = DIRECTORY_SEPARATOR; memcpy (file_name + dir_len + add_slash, base, base_len + 1); } } if (file_name == NULL) /* Out of memory. Treat the file as empty. */ cp = ""; else { int fd; /* Open the file. Reject symbolic links on platforms that support O_NOFOLLOW. This is a security feature. Without it, an attacker could retrieve parts of the contents (namely, the tail of the first line that starts with "* ") of an arbitrary file by placing a symbolic link to that file under the name "charset.alias" in some writable directory and defining the environment variable CHARSETALIASDIR to point to that directory. */ fd = open (file_name, O_RDONLY | (HAVE_WORKING_O_NOFOLLOW ? O_NOFOLLOW : 0)); if (fd < 0) /* File not found. Treat it as empty. */ cp = ""; else { FILE *fp; fp = fdopen (fd, "r"); if (fp == NULL) { /* Out of memory. Treat the file as empty. */ close (fd); cp = ""; } else { /* Parse the file's contents. */ char *res_ptr = NULL; size_t res_size = 0; for (;;) { int c; char buf1[50+1]; char buf2[50+1]; size_t l1, l2; char *old_res_ptr; c = getc (fp); if (c == EOF) break; if (c == '\n' || c == ' ' || c == '\t') continue; if (c == '#') { /* Skip comment, to end of line. */ do c = getc (fp); while (!(c == EOF || c == '\n')); if (c == EOF) break; continue; } ungetc (c, fp); if (fscanf (fp, "%50s %50s", buf1, buf2) < 2) break; l1 = strlen (buf1); l2 = strlen (buf2); old_res_ptr = res_ptr; if (res_size == 0) { res_size = l1 + 1 + l2 + 1; res_ptr = (char *) malloc (res_size + 1); } else { res_size += l1 + 1 + l2 + 1; res_ptr = (char *) realloc (res_ptr, res_size + 1); } if (res_ptr == NULL) { /* Out of memory. */ res_size = 0; free (old_res_ptr); break; } strcpy (res_ptr + res_size - (l2 + 1) - (l1 + 1), buf1); strcpy (res_ptr + res_size - (l2 + 1), buf2); } fclose (fp); if (res_size == 0) cp = ""; else { *(res_ptr + res_size) = '\0'; cp = res_ptr; } } } free (file_name); } #else # if defined DARWIN7 /* To avoid the trouble of installing a file that is shared by many GNU packages -- many packaging systems have problems with this --, simply inline the aliases here. */ cp = "ISO8859-1" "\0" "ISO-8859-1" "\0" "ISO8859-2" "\0" "ISO-8859-2" "\0" "ISO8859-4" "\0" "ISO-8859-4" "\0" "ISO8859-5" "\0" "ISO-8859-5" "\0" "ISO8859-7" "\0" "ISO-8859-7" "\0" "ISO8859-9" "\0" "ISO-8859-9" "\0" "ISO8859-13" "\0" "ISO-8859-13" "\0" "ISO8859-15" "\0" "ISO-8859-15" "\0" "KOI8-R" "\0" "KOI8-R" "\0" "KOI8-U" "\0" "KOI8-U" "\0" "CP866" "\0" "CP866" "\0" "CP949" "\0" "CP949" "\0" "CP1131" "\0" "CP1131" "\0" "CP1251" "\0" "CP1251" "\0" "eucCN" "\0" "GB2312" "\0" "GB2312" "\0" "GB2312" "\0" "eucJP" "\0" "EUC-JP" "\0" "eucKR" "\0" "EUC-KR" "\0" "Big5" "\0" "BIG5" "\0" "Big5HKSCS" "\0" "BIG5-HKSCS" "\0" "GBK" "\0" "GBK" "\0" "GB18030" "\0" "GB18030" "\0" "SJIS" "\0" "SHIFT_JIS" "\0" "ARMSCII-8" "\0" "ARMSCII-8" "\0" "PT154" "\0" "PT154" "\0" /*"ISCII-DEV" "\0" "?" "\0"*/ "*" "\0" "UTF-8" "\0"; # endif # if defined VMS /* To avoid the troubles of an extra file charset.alias_vms in the sources of many GNU packages, simply inline the aliases here. */ /* The list of encodings is taken from the OpenVMS 7.3-1 documentation "Compaq C Run-Time Library Reference Manual for OpenVMS systems" section 10.7 "Handling Different Character Sets". */ cp = "ISO8859-1" "\0" "ISO-8859-1" "\0" "ISO8859-2" "\0" "ISO-8859-2" "\0" "ISO8859-5" "\0" "ISO-8859-5" "\0" "ISO8859-7" "\0" "ISO-8859-7" "\0" "ISO8859-8" "\0" "ISO-8859-8" "\0" "ISO8859-9" "\0" "ISO-8859-9" "\0" /* Japanese */ "eucJP" "\0" "EUC-JP" "\0" "SJIS" "\0" "SHIFT_JIS" "\0" "DECKANJI" "\0" "DEC-KANJI" "\0" "SDECKANJI" "\0" "EUC-JP" "\0" /* Chinese */ "eucTW" "\0" "EUC-TW" "\0" "DECHANYU" "\0" "DEC-HANYU" "\0" "DECHANZI" "\0" "GB2312" "\0" /* Korean */ "DECKOREAN" "\0" "EUC-KR" "\0"; # endif # if defined WINDOWS_NATIVE || defined __CYGWIN__ /* To avoid the troubles of installing a separate file in the same directory as the DLL and of retrieving the DLL's directory at runtime, simply inline the aliases here. */ cp = "CP936" "\0" "GBK" "\0" "CP1361" "\0" "JOHAB" "\0" "CP20127" "\0" "ASCII" "\0" "CP20866" "\0" "KOI8-R" "\0" "CP20936" "\0" "GB2312" "\0" "CP21866" "\0" "KOI8-RU" "\0" "CP28591" "\0" "ISO-8859-1" "\0" "CP28592" "\0" "ISO-8859-2" "\0" "CP28593" "\0" "ISO-8859-3" "\0" "CP28594" "\0" "ISO-8859-4" "\0" "CP28595" "\0" "ISO-8859-5" "\0" "CP28596" "\0" "ISO-8859-6" "\0" "CP28597" "\0" "ISO-8859-7" "\0" "CP28598" "\0" "ISO-8859-8" "\0" "CP28599" "\0" "ISO-8859-9" "\0" "CP28605" "\0" "ISO-8859-15" "\0" "CP38598" "\0" "ISO-8859-8" "\0" "CP51932" "\0" "EUC-JP" "\0" "CP51936" "\0" "GB2312" "\0" "CP51949" "\0" "EUC-KR" "\0" "CP51950" "\0" "EUC-TW" "\0" "CP54936" "\0" "GB18030" "\0" "CP65001" "\0" "UTF-8" "\0"; # endif # if defined OS2 /* To avoid the troubles of installing a separate file in the same directory as the DLL and of retrieving the DLL's directory at runtime, simply inline the aliases here. */ /* The list of encodings is taken from "List of OS/2 Codepages" by Alex Taylor: . See also "IBM Globalization - Code page identifiers": . */ cp = "CP813" "\0" "ISO-8859-7" "\0" "CP878" "\0" "KOI8-R" "\0" "CP819" "\0" "ISO-8859-1" "\0" "CP912" "\0" "ISO-8859-2" "\0" "CP913" "\0" "ISO-8859-3" "\0" "CP914" "\0" "ISO-8859-4" "\0" "CP915" "\0" "ISO-8859-5" "\0" "CP916" "\0" "ISO-8859-8" "\0" "CP920" "\0" "ISO-8859-9" "\0" "CP921" "\0" "ISO-8859-13" "\0" "CP923" "\0" "ISO-8859-15" "\0" "CP954" "\0" "EUC-JP" "\0" "CP964" "\0" "EUC-TW" "\0" "CP970" "\0" "EUC-KR" "\0" "CP1089" "\0" "ISO-8859-6" "\0" "CP1208" "\0" "UTF-8" "\0" "CP1381" "\0" "GB2312" "\0" "CP1386" "\0" "GBK" "\0" "CP3372" "\0" "EUC-JP" "\0"; # endif #endif charset_aliases = cp; } return cp; } /* Determine the current locale's character encoding, and canonicalize it into one of the canonical names listed in config.charset. The result must not be freed; it is statically allocated. If the canonical name cannot be determined, the result is a non-canonical name. */ #ifdef STATIC STATIC #endif const char * locale_charset (void) { const char *codeset; const char *aliases; #if !(defined WINDOWS_NATIVE || defined OS2) # if HAVE_LANGINFO_CODESET /* Most systems support nl_langinfo (CODESET) nowadays. */ codeset = nl_langinfo (CODESET); # ifdef __CYGWIN__ /* Cygwin < 1.7 does not have locales. nl_langinfo (CODESET) always returns "US-ASCII". Return the suffix of the locale name from the environment variables (if present) or the codepage as a number. */ if (codeset != NULL && strcmp (codeset, "US-ASCII") == 0) { const char *locale; static char buf[2 + 10 + 1]; locale = getenv ("LC_ALL"); if (locale == NULL || locale[0] == '\0') { locale = getenv ("LC_CTYPE"); if (locale == NULL || locale[0] == '\0') locale = getenv ("LANG"); } if (locale != NULL && locale[0] != '\0') { /* If the locale name contains an encoding after the dot, return it. */ const char *dot = strchr (locale, '.'); if (dot != NULL) { const char *modifier; dot++; /* Look for the possible @... trailer and remove it, if any. */ modifier = strchr (dot, '@'); if (modifier == NULL) return dot; if (modifier - dot < sizeof (buf)) { memcpy (buf, dot, modifier - dot); buf [modifier - dot] = '\0'; return buf; } } } /* The Windows API has a function returning the locale's codepage as a number: GetACP(). This encoding is used by Cygwin, unless the user has set the environment variable CYGWIN=codepage:oem (which very few people do). Output directed to console windows needs to be converted (to GetOEMCP() if the console is using a raster font, or to GetConsoleOutputCP() if it is using a TrueType font). Cygwin does this conversion transparently (see winsup/cygwin/fhandler_console.cc), converting to GetConsoleOutputCP(). This leads to correct results, except when SetConsoleOutputCP has been called and a raster font is in use. */ sprintf (buf, "CP%u", GetACP ()); codeset = buf; } # endif # else /* On old systems which lack it, use setlocale or getenv. */ const char *locale = NULL; /* But most old systems don't have a complete set of locales. Some (like SunOS 4 or DJGPP) have only the C locale. Therefore we don't use setlocale here; it would return "C" when it doesn't support the locale name the user has set. */ # if 0 locale = setlocale (LC_CTYPE, NULL); # endif if (locale == NULL || locale[0] == '\0') { locale = getenv ("LC_ALL"); if (locale == NULL || locale[0] == '\0') { locale = getenv ("LC_CTYPE"); if (locale == NULL || locale[0] == '\0') locale = getenv ("LANG"); } } /* On some old systems, one used to set locale = "iso8859_1". On others, you set it to "language_COUNTRY.charset". In any case, we resolve it through the charset.alias file. */ codeset = locale; # endif #elif defined WINDOWS_NATIVE static char buf[2 + 10 + 1]; /* The Windows API has a function returning the locale's codepage as a number, but the value doesn't change according to what the 'setlocale' call specified. So we use it as a last resort, in case the string returned by 'setlocale' doesn't specify the codepage. */ char *current_locale = setlocale (LC_ALL, NULL); char *pdot; /* If they set different locales for different categories, 'setlocale' will return a semi-colon separated list of locale values. To make sure we use the correct one, we choose LC_CTYPE. */ if (strchr (current_locale, ';')) current_locale = setlocale (LC_CTYPE, NULL); pdot = strrchr (current_locale, '.'); if (pdot) sprintf (buf, "CP%s", pdot + 1); else { /* The Windows API has a function returning the locale's codepage as a number: GetACP(). When the output goes to a console window, it needs to be provided in GetOEMCP() encoding if the console is using a raster font, or in GetConsoleOutputCP() encoding if it is using a TrueType font. But in GUI programs and for output sent to files and pipes, GetACP() encoding is the best bet. */ sprintf (buf, "CP%u", GetACP ()); } codeset = buf; #elif defined OS2 const char *locale; static char buf[2 + 10 + 1]; ULONG cp[3]; ULONG cplen; codeset = NULL; /* Allow user to override the codeset, as set in the operating system, with standard language environment variables. */ locale = getenv ("LC_ALL"); if (locale == NULL || locale[0] == '\0') { locale = getenv ("LC_CTYPE"); if (locale == NULL || locale[0] == '\0') locale = getenv ("LANG"); } if (locale != NULL && locale[0] != '\0') { /* If the locale name contains an encoding after the dot, return it. */ const char *dot = strchr (locale, '.'); if (dot != NULL) { const char *modifier; dot++; /* Look for the possible @... trailer and remove it, if any. */ modifier = strchr (dot, '@'); if (modifier == NULL) return dot; if (modifier - dot < sizeof (buf)) { memcpy (buf, dot, modifier - dot); buf [modifier - dot] = '\0'; return buf; } } /* For the POSIX locale, don't use the system's codepage. */ if (strcmp (locale, "C") == 0 || strcmp (locale, "POSIX") == 0) codeset = ""; } if (codeset == NULL) { /* OS/2 has a function returning the locale's codepage as a number. */ if (DosQueryCp (sizeof (cp), cp, &cplen)) codeset = ""; else { sprintf (buf, "CP%u", cp[0]); codeset = buf; } } #endif if (codeset == NULL) /* The canonical name cannot be determined. */ codeset = ""; /* Resolve alias. */ for (aliases = get_charset_aliases (); *aliases != '\0'; aliases += strlen (aliases) + 1, aliases += strlen (aliases) + 1) if (strcmp (codeset, aliases) == 0 || (aliases[0] == '*' && aliases[1] == '\0')) { codeset = aliases + strlen (aliases) + 1; break; } /* Don't return an empty string. GNU libc and GNU libiconv interpret the empty string as denoting "the locale's character encoding", thus GNU libiconv would call this function a second time. */ if (codeset[0] == '\0') codeset = "ASCII"; #ifdef DARWIN7 /* Mac OS X sets MB_CUR_MAX to 1 when LC_ALL=C, and "UTF-8" (the default codeset) does not work when MB_CUR_MAX is 1. */ if (strcmp (codeset, "UTF-8") == 0 && MB_CUR_MAX_L (uselocale (NULL)) <= 1) codeset = "ASCII"; #endif return codeset; } gnuastro-0.2.33-8a3b/bootstrapped/lib/localcharset.h0000644000175000017500000000243213004436754017215 00000000000000/* Determine a canonical name for the current locale's character encoding. Copyright (C) 2000-2003, 2009-2016 Free Software Foundation, Inc. This file is part of the GNU CHARSET Library. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _LOCALCHARSET_H #define _LOCALCHARSET_H #ifdef __cplusplus extern "C" { #endif /* Determine the current locale's character encoding, and canonicalize it into one of the canonical names listed in config.charset. The result must not be freed; it is statically allocated. If the canonical name cannot be determined, the result is a non-canonical name. */ extern const char * locale_charset (void); #ifdef __cplusplus } #endif #endif /* _LOCALCHARSET_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/hard-locale.c0000644000175000017500000000414513004436754016722 00000000000000/* hard-locale.c -- Determine whether a locale is hard. Copyright (C) 1997-1999, 2002-2004, 2006-2007, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "hard-locale.h" #include #include #include #ifdef __GLIBC__ # define GLIBC_VERSION __GLIBC__ #elif defined __UCLIBC__ # define GLIBC_VERSION 2 #else # define GLIBC_VERSION 0 #endif /* Return true if the current CATEGORY locale is hard, i.e. if you can't get away with assuming traditional C or POSIX behavior. */ bool hard_locale (int category) { bool hard = true; char const *p = setlocale (category, NULL); if (p) { if (2 <= GLIBC_VERSION) { if (strcmp (p, "C") == 0 || strcmp (p, "POSIX") == 0) hard = false; } else { char *locale = strdup (p); if (locale) { /* Temporarily set the locale to the "C" and "POSIX" locales to find their names, so that we can determine whether one or the other is the caller's locale. */ if (((p = setlocale (category, "C")) && strcmp (p, locale) == 0) || ((p = setlocale (category, "POSIX")) && strcmp (p, locale) == 0)) hard = false; /* Restore the caller's locale. */ setlocale (category, locale); free (locale); } } } return hard; } gnuastro-0.2.33-8a3b/bootstrapped/lib/gettext.h0000644000175000017500000002364413004436754016245 00000000000000/* Convenience header for conditional use of GNU . Copyright (C) 1995-1998, 2000-2002, 2004-2006, 2009-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _LIBGETTEXT_H #define _LIBGETTEXT_H 1 /* NLS can be disabled through the configure --disable-nls option. */ #if ENABLE_NLS /* Get declarations of GNU message catalog functions. */ # include /* You can set the DEFAULT_TEXT_DOMAIN macro to specify the domain used by the gettext() and ngettext() macros. This is an alternative to calling textdomain(), and is useful for libraries. */ # ifdef DEFAULT_TEXT_DOMAIN # undef gettext # define gettext(Msgid) \ dgettext (DEFAULT_TEXT_DOMAIN, Msgid) # undef ngettext # define ngettext(Msgid1, Msgid2, N) \ dngettext (DEFAULT_TEXT_DOMAIN, Msgid1, Msgid2, N) # endif #else /* Solaris /usr/include/locale.h includes /usr/include/libintl.h, which chokes if dcgettext is defined as a macro. So include it now, to make later inclusions of a NOP. We don't include as well because people using "gettext.h" will not include , and also including would fail on SunOS 4, whereas is OK. */ #if defined(__sun) # include #endif /* Many header files from the libstdc++ coming with g++ 3.3 or newer include , which chokes if dcgettext is defined as a macro. So include it now, to make later inclusions of a NOP. */ #if defined(__cplusplus) && defined(__GNUG__) && (__GNUC__ >= 3) # include # if (__GLIBC__ >= 2 && !defined __UCLIBC__) || _GLIBCXX_HAVE_LIBINTL_H # include # endif #endif /* Disabled NLS. The casts to 'const char *' serve the purpose of producing warnings for invalid uses of the value returned from these functions. On pre-ANSI systems without 'const', the config.h file is supposed to contain "#define const". */ # undef gettext # define gettext(Msgid) ((const char *) (Msgid)) # undef dgettext # define dgettext(Domainname, Msgid) ((void) (Domainname), gettext (Msgid)) # undef dcgettext # define dcgettext(Domainname, Msgid, Category) \ ((void) (Category), dgettext (Domainname, Msgid)) # undef ngettext # define ngettext(Msgid1, Msgid2, N) \ ((N) == 1 \ ? ((void) (Msgid2), (const char *) (Msgid1)) \ : ((void) (Msgid1), (const char *) (Msgid2))) # undef dngettext # define dngettext(Domainname, Msgid1, Msgid2, N) \ ((void) (Domainname), ngettext (Msgid1, Msgid2, N)) # undef dcngettext # define dcngettext(Domainname, Msgid1, Msgid2, N, Category) \ ((void) (Category), dngettext (Domainname, Msgid1, Msgid2, N)) # undef textdomain # define textdomain(Domainname) ((const char *) (Domainname)) # undef bindtextdomain # define bindtextdomain(Domainname, Dirname) \ ((void) (Domainname), (const char *) (Dirname)) # undef bind_textdomain_codeset # define bind_textdomain_codeset(Domainname, Codeset) \ ((void) (Domainname), (const char *) (Codeset)) #endif /* Prefer gnulib's setlocale override over libintl's setlocale override. */ #ifdef GNULIB_defined_setlocale # undef setlocale # define setlocale rpl_setlocale #endif /* A pseudo function call that serves as a marker for the automated extraction of messages, but does not call gettext(). The run-time translation is done at a different place in the code. The argument, String, should be a literal string. Concatenated strings and other string expressions won't work. The macro's expansion is not parenthesized, so that it is suitable as initializer for static 'char[]' or 'const char[]' variables. */ #define gettext_noop(String) String /* The separator between msgctxt and msgid in a .mo file. */ #define GETTEXT_CONTEXT_GLUE "\004" /* Pseudo function calls, taking a MSGCTXT and a MSGID instead of just a MSGID. MSGCTXT and MSGID must be string literals. MSGCTXT should be short and rarely need to change. The letter 'p' stands for 'particular' or 'special'. */ #ifdef DEFAULT_TEXT_DOMAIN # define pgettext(Msgctxt, Msgid) \ pgettext_aux (DEFAULT_TEXT_DOMAIN, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, LC_MESSAGES) #else # define pgettext(Msgctxt, Msgid) \ pgettext_aux (NULL, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, LC_MESSAGES) #endif #define dpgettext(Domainname, Msgctxt, Msgid) \ pgettext_aux (Domainname, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, LC_MESSAGES) #define dcpgettext(Domainname, Msgctxt, Msgid, Category) \ pgettext_aux (Domainname, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, Category) #ifdef DEFAULT_TEXT_DOMAIN # define npgettext(Msgctxt, Msgid, MsgidPlural, N) \ npgettext_aux (DEFAULT_TEXT_DOMAIN, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, MsgidPlural, N, LC_MESSAGES) #else # define npgettext(Msgctxt, Msgid, MsgidPlural, N) \ npgettext_aux (NULL, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, MsgidPlural, N, LC_MESSAGES) #endif #define dnpgettext(Domainname, Msgctxt, Msgid, MsgidPlural, N) \ npgettext_aux (Domainname, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, MsgidPlural, N, LC_MESSAGES) #define dcnpgettext(Domainname, Msgctxt, Msgid, MsgidPlural, N, Category) \ npgettext_aux (Domainname, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, MsgidPlural, N, Category) #ifdef __GNUC__ __inline #else #ifdef __cplusplus inline #endif #endif static const char * pgettext_aux (const char *domain, const char *msg_ctxt_id, const char *msgid, int category) { const char *translation = dcgettext (domain, msg_ctxt_id, category); if (translation == msg_ctxt_id) return msgid; else return translation; } #ifdef __GNUC__ __inline #else #ifdef __cplusplus inline #endif #endif static const char * npgettext_aux (const char *domain, const char *msg_ctxt_id, const char *msgid, const char *msgid_plural, unsigned long int n, int category) { const char *translation = dcngettext (domain, msg_ctxt_id, msgid_plural, n, category); if (translation == msg_ctxt_id || translation == msgid_plural) return (n == 1 ? msgid : msgid_plural); else return translation; } /* The same thing extended for non-constant arguments. Here MSGCTXT and MSGID can be arbitrary expressions. But for string literals these macros are less efficient than those above. */ #include #if (((__GNUC__ >= 3 || __GNUG__ >= 2) && !defined __STRICT_ANSI__) \ /* || __STDC_VERSION__ >= 199901L */ ) # define _LIBGETTEXT_HAVE_VARIABLE_SIZE_ARRAYS 1 #else # define _LIBGETTEXT_HAVE_VARIABLE_SIZE_ARRAYS 0 #endif #if !_LIBGETTEXT_HAVE_VARIABLE_SIZE_ARRAYS #include #endif #define pgettext_expr(Msgctxt, Msgid) \ dcpgettext_expr (NULL, Msgctxt, Msgid, LC_MESSAGES) #define dpgettext_expr(Domainname, Msgctxt, Msgid) \ dcpgettext_expr (Domainname, Msgctxt, Msgid, LC_MESSAGES) #ifdef __GNUC__ __inline #else #ifdef __cplusplus inline #endif #endif static const char * dcpgettext_expr (const char *domain, const char *msgctxt, const char *msgid, int category) { size_t msgctxt_len = strlen (msgctxt) + 1; size_t msgid_len = strlen (msgid) + 1; const char *translation; #if _LIBGETTEXT_HAVE_VARIABLE_SIZE_ARRAYS char msg_ctxt_id[msgctxt_len + msgid_len]; #else char buf[1024]; char *msg_ctxt_id = (msgctxt_len + msgid_len <= sizeof (buf) ? buf : (char *) malloc (msgctxt_len + msgid_len)); if (msg_ctxt_id != NULL) #endif { int found_translation; memcpy (msg_ctxt_id, msgctxt, msgctxt_len - 1); msg_ctxt_id[msgctxt_len - 1] = '\004'; memcpy (msg_ctxt_id + msgctxt_len, msgid, msgid_len); translation = dcgettext (domain, msg_ctxt_id, category); found_translation = (translation != msg_ctxt_id); #if !_LIBGETTEXT_HAVE_VARIABLE_SIZE_ARRAYS if (msg_ctxt_id != buf) free (msg_ctxt_id); #endif if (found_translation) return translation; } return msgid; } #define npgettext_expr(Msgctxt, Msgid, MsgidPlural, N) \ dcnpgettext_expr (NULL, Msgctxt, Msgid, MsgidPlural, N, LC_MESSAGES) #define dnpgettext_expr(Domainname, Msgctxt, Msgid, MsgidPlural, N) \ dcnpgettext_expr (Domainname, Msgctxt, Msgid, MsgidPlural, N, LC_MESSAGES) #ifdef __GNUC__ __inline #else #ifdef __cplusplus inline #endif #endif static const char * dcnpgettext_expr (const char *domain, const char *msgctxt, const char *msgid, const char *msgid_plural, unsigned long int n, int category) { size_t msgctxt_len = strlen (msgctxt) + 1; size_t msgid_len = strlen (msgid) + 1; const char *translation; #if _LIBGETTEXT_HAVE_VARIABLE_SIZE_ARRAYS char msg_ctxt_id[msgctxt_len + msgid_len]; #else char buf[1024]; char *msg_ctxt_id = (msgctxt_len + msgid_len <= sizeof (buf) ? buf : (char *) malloc (msgctxt_len + msgid_len)); if (msg_ctxt_id != NULL) #endif { int found_translation; memcpy (msg_ctxt_id, msgctxt, msgctxt_len - 1); msg_ctxt_id[msgctxt_len - 1] = '\004'; memcpy (msg_ctxt_id + msgctxt_len, msgid, msgid_len); translation = dcngettext (domain, msg_ctxt_id, msgid_plural, n, category); found_translation = !(translation == msg_ctxt_id || translation == msgid_plural); #if !_LIBGETTEXT_HAVE_VARIABLE_SIZE_ARRAYS if (msg_ctxt_id != buf) free (msg_ctxt_id); #endif if (found_translation) return translation; } return (n == 1 ? msgid : msgid_plural); } #endif /* _LIBGETTEXT_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/getprogname.c0000644000175000017500000001154313004436754017057 00000000000000/* Program name management. Copyright (C) 2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include "getprogname.h" #include /* get program_invocation_name declaration */ #include /* get __argv declaration */ #ifdef _AIX # include # include # include #endif #ifdef __MVS__ # ifndef _OPEN_SYS # define _OPEN_SYS # endif # include # include #endif #ifdef __hpux # include # include # include # include #endif #include "dirname.h" #ifndef HAVE_GETPROGNAME /* not Mac OS X, FreeBSD, NetBSD, OpenBSD >= 5.4, Cygwin */ char const * getprogname (void) { # if HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME /* glibc, BeOS */ /* https://www.gnu.org/software/libc/manual/html_node/Error-Messages.html */ return program_invocation_short_name; # elif HAVE_DECL_PROGRAM_INVOCATION_NAME /* glibc, BeOS */ /* https://www.gnu.org/software/libc/manual/html_node/Error-Messages.html */ return last_component (program_invocation_name); # elif HAVE_GETEXECNAME /* Solaris */ /* http://docs.oracle.com/cd/E19253-01/816-5168/6mbb3hrb1/index.html */ const char *p = getexecname (); if (!p) p = "?"; return last_component (p); # elif HAVE_DECL___ARGV /* mingw, MSVC */ /* https://msdn.microsoft.com/en-us/library/dn727674.aspx */ const char *p = __argv && __argv[0] ? __argv[0] : "?"; return last_component (p); # elif HAVE_VAR___PROGNAME /* OpenBSD, QNX */ /* http://man.openbsd.org/style.9 */ /* http://www.qnx.de/developers/docs/6.5.0/index.jsp?topic=%2Fcom.qnx.doc.neutrino_lib_ref%2Fp%2F__progname.html */ /* Be careful to declare this only when we absolutely need it (OpenBSD 5.1), rather than when it's available. Otherwise, its mere declaration makes program_invocation_short_name malfunction (have zero length) with Fedora 25's glibc. */ extern char *__progname; const char *p = __progname; return p && p[0] ? p : "?"; # elif _AIX /* AIX */ /* Idea by Bastien ROUCARIÈS, http://lists.gnu.org/archive/html/bug-gnulib/2010-12/msg00095.html Reference: http:// ibm.biz/knowctr#ssw_aix_53/com.ibm.aix.basetechref/doc/basetrf1/getprocs.htm */ static char *p; static int first = 1; if (first) { first = 0; pid_t pid = getpid (); struct procentry64 procs; p = (0 < getprocs64 (&procs, sizeof procs, NULL, 0, &pid, 1) ? strdup (procs.pi_comm) : NULL); if (!p) p = "?"; } return p; # elif defined __hpux static char *p; static int first = 1; if (first) { first = 0; pid_t pid = getpid (); struct pst_status status; p = (0 < pstat_getproc (&status, sizeof status, 0, pid) ? strdup (status.pst_ucomm) : NULL); if (!p) p = "?"; } return p; # elif __MVS__ /* z/OS */ /* https://www.ibm.com/support/knowledgecenter/SSLTBW_2.1.0/com.ibm.zos.v2r1.bpxbd00/rtwgetp.htm */ static char *p = "?"; static int first = 1; if (first) { pid_t pid = getpid (); int token; W_PSPROC buf; first = 0; memset (&buf, 0, sizeof(buf)); buf.ps_cmdptr = (char *) malloc (buf.ps_cmdlen = PS_CMDBLEN_LONG); buf.ps_conttyptr = (char *) malloc (buf.ps_conttylen = PS_CONTTYBLEN); buf.ps_pathptr = (char *) malloc (buf.ps_pathlen = PS_PATHBLEN); if (buf.ps_cmdptr && buf.ps_conttyptr && buf.ps_pathptr) { for (token = 0; token >= 0; token = w_getpsent (token, &buf, sizeof(buf))) { if (token > 0 && buf.ps_pid == pid) { char *s = strdup (last_component (buf.ps_pathptr)); if (s) p = s; break; } } } free (buf.ps_cmdptr); free (buf.ps_conttyptr); free (buf.ps_pathptr); } return p; # else # error "getprogname module not ported to this OS" # endif } #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/getprogname.h0000644000175000017500000000216613004436754017065 00000000000000/* Program name management. Copyright (C) 2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _GL_GETPROGNAME_H #define _GL_GETPROGNAME_H #include #ifdef __cplusplus extern "C" { #endif /* Return the base name of the executing program. On native Windows this will usually end in ".exe" or ".EXE". */ #ifndef HAVE_GETPROGNAME extern char const *getprogname (void) # ifdef HAVE_DECL_PROGRAM_INVOCATION_NAME _GL_ATTRIBUTE_PURE # endif ; #endif #ifdef __cplusplus } #endif #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/stripslash.c0000644000175000017500000000304113004436754016735 00000000000000/* stripslash.c -- remove redundant trailing slashes from a file name Copyright (C) 1990, 2001, 2003-2006, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "dirname.h" /* Remove trailing slashes from FILE. Return true if a trailing slash was removed. This is useful when using file name completion from a shell that adds a "/" after directory names (such as tcsh and bash), because on symlinks to directories, several system calls have different semantics according to whether a trailing slash is present. */ bool strip_trailing_slashes (char *file) { char *base = last_component (file); char *base_lim; bool had_slash; /* last_component returns "" for file system roots, but we need to turn "///" into "/". */ if (! *base) base = file; base_lim = base + base_len (base); had_slash = (*base_lim != '\0'); *base_lim = '\0'; return had_slash; } gnuastro-0.2.33-8a3b/bootstrapped/lib/basename-lgpl.c0000644000175000017500000000406113004436754017253 00000000000000/* basename.c -- return the last element in a file name Copyright (C) 1990, 1998-2001, 2003-2006, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "dirname.h" #include /* Return the address of the last file name component of NAME. If NAME has no relative file name components because it is a file system root, return the empty string. */ char * last_component (char const *name) { char const *base = name + FILE_SYSTEM_PREFIX_LEN (name); char const *p; bool saw_slash = false; while (ISSLASH (*base)) base++; for (p = base; *p; p++) { if (ISSLASH (*p)) saw_slash = true; else if (saw_slash) { base = p; saw_slash = false; } } return (char *) base; } /* Return the length of the basename NAME. Typically NAME is the value returned by base_name or last_component. Act like strlen (NAME), except omit all trailing slashes. */ size_t base_len (char const *name) { size_t len; size_t prefix_len = FILE_SYSTEM_PREFIX_LEN (name); for (len = strlen (name); 1 < len && ISSLASH (name[len - 1]); len--) continue; if (DOUBLE_SLASH_IS_DISTINCT_ROOT && len == 1 && ISSLASH (name[0]) && ISSLASH (name[1]) && ! name[2]) return 2; if (FILE_SYSTEM_DRIVE_PREFIX_CAN_BE_RELATIVE && prefix_len && len == prefix_len && ISSLASH (name[prefix_len])) return prefix_len + 1; return len; } gnuastro-0.2.33-8a3b/bootstrapped/lib/dirname-lgpl.c0000644000175000017500000000612013004436754017115 00000000000000/* dirname.c -- return all but the last element in a file name Copyright (C) 1990, 1998, 2000-2001, 2003-2006, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "dirname.h" #include #include /* Return the length of the prefix of FILE that will be used by dir_name. If FILE is in the working directory, this returns zero even though 'dir_name (FILE)' will return ".". Works properly even if there are trailing slashes (by effectively ignoring them). */ size_t dir_len (char const *file) { size_t prefix_length = FILE_SYSTEM_PREFIX_LEN (file); size_t length; /* Advance prefix_length beyond important leading slashes. */ prefix_length += (prefix_length != 0 ? (FILE_SYSTEM_DRIVE_PREFIX_CAN_BE_RELATIVE && ISSLASH (file[prefix_length])) : (ISSLASH (file[0]) ? ((DOUBLE_SLASH_IS_DISTINCT_ROOT && ISSLASH (file[1]) && ! ISSLASH (file[2]) ? 2 : 1)) : 0)); /* Strip the basename and any redundant slashes before it. */ for (length = last_component (file) - file; prefix_length < length; length--) if (! ISSLASH (file[length - 1])) break; return length; } /* In general, we can't use the builtin 'dirname' function if available, since it has different meanings in different environments. In some environments the builtin 'dirname' modifies its argument. Return the leading directories part of FILE, allocated with malloc. Works properly even if there are trailing slashes (by effectively ignoring them). Return NULL on failure. If lstat (FILE) would succeed, then { chdir (dir_name (FILE)); lstat (base_name (FILE)); } will access the same file. Likewise, if the sequence { chdir (dir_name (FILE)); rename (base_name (FILE), "foo"); } succeeds, you have renamed FILE to "foo" in the same directory FILE was in. */ char * mdir_name (char const *file) { size_t length = dir_len (file); bool append_dot = (length == 0 || (FILE_SYSTEM_DRIVE_PREFIX_CAN_BE_RELATIVE && length == FILE_SYSTEM_PREFIX_LEN (file) && file[2] != '\0' && ! ISSLASH (file[2]))); char *dir = malloc (length + append_dot + 1); if (!dir) return NULL; memcpy (dir, file, length); if (append_dot) dir[length++] = '.'; dir[length] = '\0'; return dir; } gnuastro-0.2.33-8a3b/bootstrapped/lib/c-ctype.c0000644000175000017500000000012213004436754016102 00000000000000#include #define C_CTYPE_INLINE _GL_EXTERN_INLINE #include "c-ctype.h" gnuastro-0.2.33-8a3b/bootstrapped/lib/c-ctype.h0000644000175000017500000002240613004436754016120 00000000000000/* Character handling in C locale. These functions work like the corresponding functions in , except that they have the C (POSIX) locale hardwired, whereas the functions' behaviour depends on the current locale set via setlocale. Copyright (C) 2000-2003, 2006, 2008-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef C_CTYPE_H #define C_CTYPE_H #include #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef C_CTYPE_INLINE # define C_CTYPE_INLINE _GL_INLINE #endif #ifdef __cplusplus extern "C" { #endif /* The functions defined in this file assume the "C" locale and a character set without diacritics (ASCII-US or EBCDIC-US or something like that). Even if the "C" locale on a particular system is an extension of the ASCII character set (like on BeOS, where it is UTF-8, or on AmigaOS, where it is ISO-8859-1), the functions in this file recognize only the ASCII characters. */ #if (' ' == 32) && ('!' == 33) && ('"' == 34) && ('#' == 35) \ && ('%' == 37) && ('&' == 38) && ('\'' == 39) && ('(' == 40) \ && (')' == 41) && ('*' == 42) && ('+' == 43) && (',' == 44) \ && ('-' == 45) && ('.' == 46) && ('/' == 47) && ('0' == 48) \ && ('1' == 49) && ('2' == 50) && ('3' == 51) && ('4' == 52) \ && ('5' == 53) && ('6' == 54) && ('7' == 55) && ('8' == 56) \ && ('9' == 57) && (':' == 58) && (';' == 59) && ('<' == 60) \ && ('=' == 61) && ('>' == 62) && ('?' == 63) && ('A' == 65) \ && ('B' == 66) && ('C' == 67) && ('D' == 68) && ('E' == 69) \ && ('F' == 70) && ('G' == 71) && ('H' == 72) && ('I' == 73) \ && ('J' == 74) && ('K' == 75) && ('L' == 76) && ('M' == 77) \ && ('N' == 78) && ('O' == 79) && ('P' == 80) && ('Q' == 81) \ && ('R' == 82) && ('S' == 83) && ('T' == 84) && ('U' == 85) \ && ('V' == 86) && ('W' == 87) && ('X' == 88) && ('Y' == 89) \ && ('Z' == 90) && ('[' == 91) && ('\\' == 92) && (']' == 93) \ && ('^' == 94) && ('_' == 95) && ('a' == 97) && ('b' == 98) \ && ('c' == 99) && ('d' == 100) && ('e' == 101) && ('f' == 102) \ && ('g' == 103) && ('h' == 104) && ('i' == 105) && ('j' == 106) \ && ('k' == 107) && ('l' == 108) && ('m' == 109) && ('n' == 110) \ && ('o' == 111) && ('p' == 112) && ('q' == 113) && ('r' == 114) \ && ('s' == 115) && ('t' == 116) && ('u' == 117) && ('v' == 118) \ && ('w' == 119) && ('x' == 120) && ('y' == 121) && ('z' == 122) \ && ('{' == 123) && ('|' == 124) && ('}' == 125) && ('~' == 126) /* The character set is ASCII or one of its variants or extensions, not EBCDIC. Testing the value of '\n' and '\r' is not relevant. */ # define C_CTYPE_ASCII 1 #elif ! (' ' == '\x40' && '0' == '\xf0' \ && 'A' == '\xc1' && 'J' == '\xd1' && 'S' == '\xe2' \ && 'a' == '\x81' && 'j' == '\x91' && 's' == '\xa2') # error "Only ASCII and EBCDIC are supported" #endif #if 'A' < 0 # error "EBCDIC and char is signed -- not supported" #endif /* Cases for control characters. */ #define _C_CTYPE_CNTRL \ case '\a': case '\b': case '\f': case '\n': \ case '\r': case '\t': case '\v': \ _C_CTYPE_OTHER_CNTRL /* ASCII control characters other than those with \-letter escapes. */ #if C_CTYPE_ASCII # define _C_CTYPE_OTHER_CNTRL \ case '\x00': case '\x01': case '\x02': case '\x03': \ case '\x04': case '\x05': case '\x06': case '\x0e': \ case '\x0f': case '\x10': case '\x11': case '\x12': \ case '\x13': case '\x14': case '\x15': case '\x16': \ case '\x17': case '\x18': case '\x19': case '\x1a': \ case '\x1b': case '\x1c': case '\x1d': case '\x1e': \ case '\x1f': case '\x7f' #else /* Use EBCDIC code page 1047's assignments for ASCII control chars; assume all EBCDIC code pages agree about these assignments. */ # define _C_CTYPE_OTHER_CNTRL \ case '\x00': case '\x01': case '\x02': case '\x03': \ case '\x07': case '\x0e': case '\x0f': case '\x10': \ case '\x11': case '\x12': case '\x13': case '\x18': \ case '\x19': case '\x1c': case '\x1d': case '\x1e': \ case '\x1f': case '\x26': case '\x27': case '\x2d': \ case '\x2e': case '\x32': case '\x37': case '\x3c': \ case '\x3d': case '\x3f' #endif /* Cases for lowercase hex letters, and lowercase letters, all offset by N. */ #define _C_CTYPE_LOWER_A_THRU_F_N(n) \ case 'a' + (n): case 'b' + (n): case 'c' + (n): case 'd' + (n): \ case 'e' + (n): case 'f' + (n) #define _C_CTYPE_LOWER_N(n) \ _C_CTYPE_LOWER_A_THRU_F_N(n): \ case 'g' + (n): case 'h' + (n): case 'i' + (n): case 'j' + (n): \ case 'k' + (n): case 'l' + (n): case 'm' + (n): case 'n' + (n): \ case 'o' + (n): case 'p' + (n): case 'q' + (n): case 'r' + (n): \ case 's' + (n): case 't' + (n): case 'u' + (n): case 'v' + (n): \ case 'w' + (n): case 'x' + (n): case 'y' + (n): case 'z' + (n) /* Cases for hex letters, digits, lower, punct, and upper. */ #define _C_CTYPE_A_THRU_F \ _C_CTYPE_LOWER_A_THRU_F_N (0): \ _C_CTYPE_LOWER_A_THRU_F_N ('A' - 'a') #define _C_CTYPE_DIGIT \ case '0': case '1': case '2': case '3': \ case '4': case '5': case '6': case '7': \ case '8': case '9' #define _C_CTYPE_LOWER _C_CTYPE_LOWER_N (0) #define _C_CTYPE_PUNCT \ case '!': case '"': case '#': case '$': \ case '%': case '&': case '\'': case '(': \ case ')': case '*': case '+': case ',': \ case '-': case '.': case '/': case ':': \ case ';': case '<': case '=': case '>': \ case '?': case '@': case '[': case '\\': \ case ']': case '^': case '_': case '`': \ case '{': case '|': case '}': case '~' #define _C_CTYPE_UPPER _C_CTYPE_LOWER_N ('A' - 'a') /* Function definitions. */ /* Unlike the functions in , which require an argument in the range of the 'unsigned char' type, the functions here operate on values that are in the 'unsigned char' range or in the 'char' range. In other words, when you have a 'char' value, you need to cast it before using it as argument to a function: const char *s = ...; if (isalpha ((unsigned char) *s)) ... but you don't need to cast it for the functions defined in this file: const char *s = ...; if (c_isalpha (*s)) ... */ C_CTYPE_INLINE bool c_isalnum (int c) { switch (c) { _C_CTYPE_DIGIT: _C_CTYPE_LOWER: _C_CTYPE_UPPER: return true; default: return false; } } C_CTYPE_INLINE bool c_isalpha (int c) { switch (c) { _C_CTYPE_LOWER: _C_CTYPE_UPPER: return true; default: return false; } } /* The function isascii is not locale dependent. Its use in EBCDIC is questionable. */ C_CTYPE_INLINE bool c_isascii (int c) { switch (c) { case ' ': _C_CTYPE_CNTRL: _C_CTYPE_DIGIT: _C_CTYPE_LOWER: _C_CTYPE_PUNCT: _C_CTYPE_UPPER: return true; default: return false; } } C_CTYPE_INLINE bool c_isblank (int c) { return c == ' ' || c == '\t'; } C_CTYPE_INLINE bool c_iscntrl (int c) { switch (c) { _C_CTYPE_CNTRL: return true; default: return false; } } C_CTYPE_INLINE bool c_isdigit (int c) { switch (c) { _C_CTYPE_DIGIT: return true; default: return false; } } C_CTYPE_INLINE bool c_isgraph (int c) { switch (c) { _C_CTYPE_DIGIT: _C_CTYPE_LOWER: _C_CTYPE_PUNCT: _C_CTYPE_UPPER: return true; default: return false; } } C_CTYPE_INLINE bool c_islower (int c) { switch (c) { _C_CTYPE_LOWER: return true; default: return false; } } C_CTYPE_INLINE bool c_isprint (int c) { switch (c) { case ' ': _C_CTYPE_DIGIT: _C_CTYPE_LOWER: _C_CTYPE_PUNCT: _C_CTYPE_UPPER: return true; default: return false; } } C_CTYPE_INLINE bool c_ispunct (int c) { switch (c) { _C_CTYPE_PUNCT: return true; default: return false; } } C_CTYPE_INLINE bool c_isspace (int c) { switch (c) { case ' ': case '\t': case '\n': case '\v': case '\f': case '\r': return true; default: return false; } } C_CTYPE_INLINE bool c_isupper (int c) { switch (c) { _C_CTYPE_UPPER: return true; default: return false; } } C_CTYPE_INLINE bool c_isxdigit (int c) { switch (c) { _C_CTYPE_DIGIT: _C_CTYPE_A_THRU_F: return true; default: return false; } } C_CTYPE_INLINE int c_tolower (int c) { switch (c) { _C_CTYPE_UPPER: return c - 'A' + 'a'; default: return c; } } C_CTYPE_INLINE int c_toupper (int c) { switch (c) { _C_CTYPE_LOWER: return c - 'a' + 'A'; default: return c; } } #ifdef __cplusplus } #endif _GL_INLINE_HEADER_END #endif /* C_CTYPE_H */ gnuastro-0.2.33-8a3b/bootstrapped/lib/argp-xinl.c0000644000175000017500000000256513004436754016454 00000000000000/* Real definitions for extern inline functions in argp.h Copyright (C) 1997-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifdef HAVE_CONFIG_H # include #endif #if defined _LIBC || defined HAVE_FEATURES_H # include #endif #ifndef __USE_EXTERN_INLINES # define __USE_EXTERN_INLINES 1 #endif #ifdef _LIBC # define ARGP_EI #else # define ARGP_EI _GL_EXTERN_INLINE #endif #undef __OPTIMIZE__ #define __OPTIMIZE__ 1 #include "argp.h" /* Add weak aliases. */ #if _LIBC - 0 && defined (weak_alias) weak_alias (__argp_usage, argp_usage) weak_alias (__option_is_short, _option_is_short) weak_alias (__option_is_end, _option_is_end) #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/argp-pvh.c0000644000175000017500000000253513004436754016274 00000000000000/* Default definition for ARGP_PROGRAM_VERSION_HOOK. Copyright (C) 1996-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifdef HAVE_CONFIG_H # include #endif #include "argp.h" /* If set by the user program to a non-zero value, then a default option --version is added (unless the ARGP_NO_HELP flag is used), which calls this function with a stream to print the version to and a pointer to the current parsing state, and then exits (unless the ARGP_NO_EXIT flag is used). This variable takes precedent over ARGP_PROGRAM_VERSION. */ void (*argp_program_version_hook) (FILE *stream, struct argp_state *state) = NULL; gnuastro-0.2.33-8a3b/bootstrapped/lib/argp-pv.c0000644000175000017500000000304113004436754016115 00000000000000/* Default definition for ARGP_PROGRAM_VERSION. Copyright (C) 1996-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* If set by the user program to a non-zero value, then a default option --version is added (unless the ARGP_NO_HELP flag is used), which will print this string followed by a newline and exit (unless the ARGP_NO_EXIT flag is used). Overridden by ARGP_PROGRAM_VERSION_HOOK. */ const char *argp_program_version /* This variable should be zero-initialized. On most systems, putting it into BSS is sufficient. Not so on Mac OS X 10.3 and 10.4, see . */ #if defined __ELF__ /* On ELF systems, variables in BSS behave well. */ #else = (const char *) 0 #endif ; gnuastro-0.2.33-8a3b/bootstrapped/lib/argp-pin.c0000644000175000017500000000172413004436754016264 00000000000000/* Full and short program names for argp module Copyright (C) 2005, 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifdef HAVE_CONFIG_H # include #endif #ifndef HAVE_PROGRAM_INVOCATION_SHORT_NAME char *program_invocation_short_name = 0; #endif #ifndef HAVE_PROGRAM_INVOCATION_NAME char *program_invocation_name = 0; #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/argp-parse.c0000644000175000017500000007565413004436754016625 00000000000000/* Hierarchical argument parsing, layered over getopt Copyright (C) 1995-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifdef HAVE_CONFIG_H # include #endif #include #include #include #include #include #include #include #include #include #ifdef _LIBC # include # undef dgettext # define dgettext(domain, msgid) \ __dcgettext (domain, msgid, LC_MESSAGES) #else # include "gettext.h" #endif #define N_(msgid) msgid #include "argp.h" #include "argp-namefrob.h" #define alignto(n, d) ((((n) + (d) - 1) / (d)) * (d)) /* Getopt return values. */ #define KEY_END (-1) /* The end of the options. */ #define KEY_ARG 1 /* A non-option argument. */ #define KEY_ERR '?' /* An error parsing the options. */ /* The meta-argument used to prevent any further arguments being interpreted as options. */ #define QUOTE "--" /* The number of bits we steal in a long-option value for our own use. */ #define GROUP_BITS CHAR_BIT /* The number of bits available for the user value. */ #define USER_BITS ((sizeof ((struct option *)0)->val * CHAR_BIT) - GROUP_BITS) #define USER_MASK ((1 << USER_BITS) - 1) /* EZ alias for ARGP_ERR_UNKNOWN. */ #define EBADKEY ARGP_ERR_UNKNOWN /* Default options. */ /* When argp is given the --HANG switch, _ARGP_HANG is set and argp will sleep for one second intervals, decrementing _ARGP_HANG until it's zero. Thus you can force the program to continue by attaching a debugger and setting it to 0 yourself. */ static volatile int _argp_hang; #define OPT_PROGNAME -2 #define OPT_USAGE -3 #define OPT_HANG -4 static const struct argp_option argp_default_options[] = { {"help", '?', 0, 0, N_("give this help list"), -1}, {"usage", OPT_USAGE, 0, 0, N_("give a short usage message"), 0}, {"program-name",OPT_PROGNAME, N_("NAME"), OPTION_HIDDEN, N_("set the program name"), 0}, {"HANG", OPT_HANG, N_("SECS"), OPTION_ARG_OPTIONAL | OPTION_HIDDEN, N_("hang for SECS seconds (default 3600)"), 0}, {NULL, 0, 0, 0, NULL, 0} }; static error_t argp_default_parser (int key, char *arg, struct argp_state *state) { switch (key) { case '?': __argp_state_help (state, state->out_stream, ARGP_HELP_STD_HELP); break; case OPT_USAGE: __argp_state_help (state, state->out_stream, ARGP_HELP_USAGE | ARGP_HELP_EXIT_OK); break; case OPT_PROGNAME: /* Set the program name. */ #if defined _LIBC || HAVE_DECL_PROGRAM_INVOCATION_NAME program_invocation_name = arg; #endif /* [Note that some systems only have PROGRAM_INVOCATION_SHORT_NAME (aka __PROGNAME), in which case, PROGRAM_INVOCATION_NAME is just defined to be that, so we have to be a bit careful here.] */ /* Update what we use for messages. */ state->name = __argp_base_name (arg); #if defined _LIBC || HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME program_invocation_short_name = state->name; #endif if ((state->flags & (ARGP_PARSE_ARGV0 | ARGP_NO_ERRS)) == ARGP_PARSE_ARGV0) /* Update what getopt uses too. */ state->argv[0] = arg; break; case OPT_HANG: _argp_hang = atoi (arg ? arg : "3600"); while (_argp_hang-- > 0) __sleep (1); break; default: return EBADKEY; } return 0; } static const struct argp argp_default_argp = {argp_default_options, &argp_default_parser, NULL, NULL, NULL, NULL, "libc"}; static const struct argp_option argp_version_options[] = { {"version", 'V', 0, 0, N_("print program version"), -1}, {NULL, 0, 0, 0, NULL, 0} }; static error_t argp_version_parser (int key, char *arg, struct argp_state *state) { switch (key) { case 'V': if (argp_program_version_hook) (*argp_program_version_hook) (state->out_stream, state); else if (argp_program_version) fprintf (state->out_stream, "%s\n", argp_program_version); else __argp_error (state, "%s", dgettext (state->root_argp->argp_domain, "(PROGRAM ERROR) No version known!?")); if (! (state->flags & ARGP_NO_EXIT)) exit (0); break; default: return EBADKEY; } return 0; } static const struct argp argp_version_argp = {argp_version_options, &argp_version_parser, NULL, NULL, NULL, NULL, "libc"}; /* Returns the offset into the getopt long options array LONG_OPTIONS of a long option with called NAME, or -1 if none is found. Passing NULL as NAME will return the number of options. */ static int find_long_option (struct option *long_options, const char *name) { struct option *l = long_options; while (l->name != NULL) if (name != NULL && strcmp (l->name, name) == 0) return l - long_options; else l++; if (name == NULL) return l - long_options; else return -1; } /* The state of a "group" during parsing. Each group corresponds to a particular argp structure from the tree of such descending from the top level argp passed to argp_parse. */ struct group { /* This group's parsing function. */ argp_parser_t parser; /* Which argp this group is from. */ const struct argp *argp; /* Points to the point in SHORT_OPTS corresponding to the end of the short options for this group. We use it to determine from which group a particular short options is from. */ char *short_end; /* The number of non-option args successfully handled by this parser. */ unsigned args_processed; /* This group's parser's parent's group. */ struct group *parent; unsigned parent_index; /* And the our position in the parent. */ /* These fields are swapped into and out of the state structure when calling this group's parser. */ void *input, **child_inputs; void *hook; }; /* Call GROUP's parser with KEY and ARG, swapping any group-specific info from STATE before calling, and back into state afterwards. If GROUP has no parser, EBADKEY is returned. */ static error_t group_parse (struct group *group, struct argp_state *state, int key, char *arg) { if (group->parser) { error_t err; state->hook = group->hook; state->input = group->input; state->child_inputs = group->child_inputs; state->arg_num = group->args_processed; err = (*group->parser)(key, arg, state); group->hook = state->hook; return err; } else return EBADKEY; } struct parser { const struct argp *argp; /* SHORT_OPTS is the getopt short options string for the union of all the groups of options. */ char *short_opts; /* LONG_OPTS is the array of getop long option structures for the union of all the groups of options. */ struct option *long_opts; /* OPT_DATA is the getopt data used for the re-entrant getopt. */ struct _getopt_data opt_data; /* States of the various parsing groups. */ struct group *groups; /* The end of the GROUPS array. */ struct group *egroup; /* A vector containing storage for the CHILD_INPUTS field in all groups. */ void **child_inputs; /* True if we think using getopt is still useful; if false, then remaining arguments are just passed verbatim with ARGP_KEY_ARG. This is cleared whenever getopt returns KEY_END, but may be set again if the user moves the next argument pointer backwards. */ int try_getopt; /* State block supplied to parsing routines. */ struct argp_state state; /* Memory used by this parser. */ void *storage; }; /* The next usable entries in the various parser tables being filled in by convert_options. */ struct parser_convert_state { struct parser *parser; char *short_end; struct option *long_end; void **child_inputs_end; }; /* Converts all options in ARGP (which is put in GROUP) and ancestors into getopt options stored in SHORT_OPTS and LONG_OPTS; SHORT_END and CVT->LONG_END are the points at which new options are added. Returns the next unused group entry. CVT holds state used during the conversion. */ static struct group * convert_options (const struct argp *argp, struct group *parent, unsigned parent_index, struct group *group, struct parser_convert_state *cvt) { /* REAL is the most recent non-alias value of OPT. */ const struct argp_option *real = argp->options; const struct argp_child *children = argp->children; if (real || argp->parser) { const struct argp_option *opt; if (real) for (opt = real; !__option_is_end (opt); opt++) { if (! (opt->flags & OPTION_ALIAS)) /* OPT isn't an alias, so we can use values from it. */ real = opt; if (! (real->flags & OPTION_DOC)) /* A real option (not just documentation). */ { if (__option_is_short (opt)) /* OPT can be used as a short option. */ { *cvt->short_end++ = opt->key; if (real->arg) { *cvt->short_end++ = ':'; if (real->flags & OPTION_ARG_OPTIONAL) *cvt->short_end++ = ':'; } *cvt->short_end = '\0'; /* keep 0 terminated */ } if (opt->name && find_long_option (cvt->parser->long_opts, opt->name) < 0) /* OPT can be used as a long option. */ { cvt->long_end->name = opt->name; cvt->long_end->has_arg = (real->arg ? (real->flags & OPTION_ARG_OPTIONAL ? optional_argument : required_argument) : no_argument); cvt->long_end->flag = 0; /* we add a disambiguating code to all the user's values (which is removed before we actually call the function to parse the value); this means that the user loses use of the high 8 bits in all his values (the sign of the lower bits is preserved however)... */ cvt->long_end->val = ((opt->key ? opt->key : real->key) & USER_MASK) + (((group - cvt->parser->groups) + 1) << USER_BITS); /* Keep the LONG_OPTS list terminated. */ (++cvt->long_end)->name = NULL; } } } group->parser = argp->parser; group->argp = argp; group->short_end = cvt->short_end; group->args_processed = 0; group->parent = parent; group->parent_index = parent_index; group->input = 0; group->hook = 0; group->child_inputs = 0; if (children) /* Assign GROUP's CHILD_INPUTS field some space from CVT->child_inputs_end.*/ { unsigned num_children = 0; while (children[num_children].argp) num_children++; group->child_inputs = cvt->child_inputs_end; cvt->child_inputs_end += num_children; } parent = group++; } else parent = 0; if (children) { unsigned index = 0; while (children->argp) group = convert_options (children++->argp, parent, index++, group, cvt); } return group; } /* Find the merged set of getopt options, with keys appropriately prefixed. */ static void parser_convert (struct parser *parser, const struct argp *argp, int flags) { struct parser_convert_state cvt; cvt.parser = parser; cvt.short_end = parser->short_opts; cvt.long_end = parser->long_opts; cvt.child_inputs_end = parser->child_inputs; if (flags & ARGP_IN_ORDER) *cvt.short_end++ = '-'; else if (flags & ARGP_NO_ARGS) *cvt.short_end++ = '+'; *cvt.short_end = '\0'; cvt.long_end->name = NULL; parser->argp = argp; if (argp) parser->egroup = convert_options (argp, 0, 0, parser->groups, &cvt); else parser->egroup = parser->groups; /* No parsers at all! */ } /* Lengths of various parser fields which we will allocated. */ struct parser_sizes { size_t short_len; /* Getopt short options string. */ size_t long_len; /* Getopt long options vector. */ size_t num_groups; /* Group structures we allocate. */ size_t num_child_inputs; /* Child input slots. */ }; /* For ARGP, increments the NUM_GROUPS field in SZS by the total number of argp structures descended from it, and the SHORT_LEN & LONG_LEN fields by the maximum lengths of the resulting merged getopt short options string and long-options array, respectively. */ static void calc_sizes (const struct argp *argp, struct parser_sizes *szs) { const struct argp_child *child = argp->children; const struct argp_option *opt = argp->options; if (opt || argp->parser) { szs->num_groups++; if (opt) { int num_opts = 0; while (!__option_is_end (opt++)) num_opts++; szs->short_len += num_opts * 3; /* opt + up to 2 ':'s */ szs->long_len += num_opts; } } if (child) while (child->argp) { calc_sizes ((child++)->argp, szs); szs->num_child_inputs++; } } /* Initializes PARSER to parse ARGP in a manner described by FLAGS. */ static error_t parser_init (struct parser *parser, const struct argp *argp, int argc, char **argv, int flags, void *input) { error_t err = 0; struct group *group; struct parser_sizes szs; struct _getopt_data opt_data = _GETOPT_DATA_INITIALIZER; char *storage; size_t glen, gsum; size_t clen, csum; size_t llen, lsum; size_t slen, ssum; szs.short_len = (flags & ARGP_NO_ARGS) ? 0 : 1; szs.long_len = 0; szs.num_groups = 0; szs.num_child_inputs = 0; if (argp) calc_sizes (argp, &szs); /* Lengths of the various bits of storage used by PARSER. */ glen = (szs.num_groups + 1) * sizeof (struct group); clen = szs.num_child_inputs * sizeof (void *); llen = (szs.long_len + 1) * sizeof (struct option); slen = szs.short_len + 1; /* Sums of previous lengths, properly aligned. There's no need to align gsum, since struct group is aligned at least as strictly as void * (since it contains a void * member). And there's no need to align lsum, since struct option is aligned at least as strictly as char. */ gsum = glen; csum = alignto (gsum + clen, alignof (struct option)); lsum = csum + llen; ssum = lsum + slen; parser->storage = malloc (ssum); if (! parser->storage) return ENOMEM; storage = parser->storage; parser->groups = parser->storage; parser->child_inputs = (void **) (storage + gsum); parser->long_opts = (struct option *) (storage + csum); parser->short_opts = storage + lsum; parser->opt_data = opt_data; memset (parser->child_inputs, 0, clen); parser_convert (parser, argp, flags); memset (&parser->state, 0, sizeof (struct argp_state)); parser->state.root_argp = parser->argp; parser->state.argc = argc; parser->state.argv = argv; parser->state.flags = flags; parser->state.err_stream = stderr; parser->state.out_stream = stdout; parser->state.next = 0; /* Tell getopt to initialize. */ parser->state.pstate = parser; parser->try_getopt = 1; /* Call each parser for the first time, giving it a chance to propagate values to child parsers. */ if (parser->groups < parser->egroup) parser->groups->input = input; for (group = parser->groups; group < parser->egroup && (!err || err == EBADKEY); group++) { if (group->parent) /* If a child parser, get the initial input value from the parent. */ group->input = group->parent->child_inputs[group->parent_index]; if (!group->parser && group->argp->children && group->argp->children->argp) /* For the special case where no parsing function is supplied for an argp, propagate its input to its first child, if any (this just makes very simple wrapper argps more convenient). */ group->child_inputs[0] = group->input; err = group_parse (group, &parser->state, ARGP_KEY_INIT, 0); } if (err == EBADKEY) err = 0; /* Some parser didn't understand. */ if (err) return err; if (parser->state.flags & ARGP_NO_ERRS) { parser->opt_data.opterr = 0; if (parser->state.flags & ARGP_PARSE_ARGV0) /* getopt always skips ARGV[0], so we have to fake it out. As long as OPTERR is 0, then it shouldn't actually try to access it. */ parser->state.argv--, parser->state.argc++; } else parser->opt_data.opterr = 1; /* Print error messages. */ if (parser->state.argv == argv && argv[0]) /* There's an argv[0]; use it for messages. */ parser->state.name = __argp_base_name (argv[0]); else parser->state.name = __argp_short_program_name (); return 0; } /* Free any storage consumed by PARSER (but not PARSER itself). */ static error_t parser_finalize (struct parser *parser, error_t err, int arg_ebadkey, int *end_index) { struct group *group; if (err == EBADKEY && arg_ebadkey) /* Suppress errors generated by unparsed arguments. */ err = 0; if (! err) { if (parser->state.next == parser->state.argc) /* We successfully parsed all arguments! Call all the parsers again, just a few more times... */ { for (group = parser->groups; group < parser->egroup && (!err || err==EBADKEY); group++) if (group->args_processed == 0) err = group_parse (group, &parser->state, ARGP_KEY_NO_ARGS, 0); for (group = parser->egroup - 1; group >= parser->groups && (!err || err==EBADKEY); group--) err = group_parse (group, &parser->state, ARGP_KEY_END, 0); if (err == EBADKEY) err = 0; /* Some parser didn't understand. */ /* Tell the user that all arguments are parsed. */ if (end_index) *end_index = parser->state.next; } else if (end_index) /* Return any remaining arguments to the user. */ *end_index = parser->state.next; else /* No way to return the remaining arguments, they must be bogus. */ { if (!(parser->state.flags & ARGP_NO_ERRS) && parser->state.err_stream) fprintf (parser->state.err_stream, dgettext (parser->argp->argp_domain, "%s: Too many arguments\n"), parser->state.name); err = EBADKEY; } } /* Okay, we're all done, with either an error or success; call the parsers to indicate which one. */ if (err) { /* Maybe print an error message. */ if (err == EBADKEY) /* An appropriate message describing what the error was should have been printed earlier. */ __argp_state_help (&parser->state, parser->state.err_stream, ARGP_HELP_STD_ERR); /* Since we didn't exit, give each parser an error indication. */ for (group = parser->groups; group < parser->egroup; group++) group_parse (group, &parser->state, ARGP_KEY_ERROR, 0); } else /* Notify parsers of success, and propagate back values from parsers. */ { /* We pass over the groups in reverse order so that child groups are given a chance to do there processing before passing back a value to the parent. */ for (group = parser->egroup - 1 ; group >= parser->groups && (!err || err == EBADKEY) ; group--) err = group_parse (group, &parser->state, ARGP_KEY_SUCCESS, 0); if (err == EBADKEY) err = 0; /* Some parser didn't understand. */ } /* Call parsers once more, to do any final cleanup. Errors are ignored. */ for (group = parser->egroup - 1; group >= parser->groups; group--) group_parse (group, &parser->state, ARGP_KEY_FINI, 0); if (err == EBADKEY) err = EINVAL; free (parser->storage); return err; } /* Call the user parsers to parse the non-option argument VAL, at the current position, returning any error. The state NEXT pointer is assumed to have been adjusted (by getopt) to point after this argument; this function will adjust it correctly to reflect however many args actually end up being consumed. */ static error_t parser_parse_arg (struct parser *parser, char *val) { /* Save the starting value of NEXT, first adjusting it so that the arg we're parsing is again the front of the arg vector. */ int index = --parser->state.next; error_t err = EBADKEY; struct group *group; int key = 0; /* Which of ARGP_KEY_ARG[S] we used. */ /* Try to parse the argument in each parser. */ for (group = parser->groups ; group < parser->egroup && err == EBADKEY ; group++) { parser->state.next++; /* For ARGP_KEY_ARG, consume the arg. */ key = ARGP_KEY_ARG; err = group_parse (group, &parser->state, key, val); if (err == EBADKEY) /* This parser doesn't like ARGP_KEY_ARG; try ARGP_KEY_ARGS instead. */ { parser->state.next--; /* For ARGP_KEY_ARGS, put back the arg. */ key = ARGP_KEY_ARGS; err = group_parse (group, &parser->state, key, 0); } } if (! err) { if (key == ARGP_KEY_ARGS) /* The default for ARGP_KEY_ARGS is to assume that if NEXT isn't changed by the user, *all* arguments should be considered consumed. */ parser->state.next = parser->state.argc; if (parser->state.next > index) /* Remember that we successfully processed a non-option argument -- but only if the user hasn't gotten tricky and set the clock back. */ (--group)->args_processed += (parser->state.next - index); else /* The user wants to reparse some args, give getopt another try. */ parser->try_getopt = 1; } return err; } /* Call the user parsers to parse the option OPT, with argument VAL, at the current position, returning any error. */ static error_t parser_parse_opt (struct parser *parser, int opt, char *val) { /* The group key encoded in the high bits; 0 for short opts or group_number + 1 for long opts. */ int group_key = opt >> USER_BITS; error_t err = EBADKEY; if (group_key == 0) /* A short option. By comparing OPT's position in SHORT_OPTS to the various starting positions in each group's SHORT_END field, we can determine which group OPT came from. */ { struct group *group; char *short_index = strchr (parser->short_opts, opt); if (short_index) for (group = parser->groups; group < parser->egroup; group++) if (group->short_end > short_index) { err = group_parse (group, &parser->state, opt, parser->opt_data.optarg); break; } } else /* A long option. We use shifts instead of masking for extracting the user value in order to preserve the sign. */ err = group_parse (&parser->groups[group_key - 1], &parser->state, (opt << GROUP_BITS) >> GROUP_BITS, parser->opt_data.optarg); if (err == EBADKEY) /* At least currently, an option not recognized is an error in the parser, because we pre-compute which parser is supposed to deal with each option. */ { static const char bad_key_err[] = N_("(PROGRAM ERROR) Option should have been recognized!?"); if (group_key == 0) __argp_error (&parser->state, "-%c: %s", opt, dgettext (parser->argp->argp_domain, bad_key_err)); else { struct option *long_opt = parser->long_opts; while (long_opt->val != opt && long_opt->name) long_opt++; __argp_error (&parser->state, "--%s: %s", long_opt->name ? long_opt->name : "???", dgettext (parser->argp->argp_domain, bad_key_err)); } } return err; } /* Parse the next argument in PARSER (as indicated by PARSER->state.next). Any error from the parsers is returned, and *ARGP_EBADKEY indicates whether a value of EBADKEY is due to an unrecognized argument (which is generally not fatal). */ static error_t parser_parse_next (struct parser *parser, int *arg_ebadkey) { int opt; error_t err = 0; if (parser->state.quoted && parser->state.next < parser->state.quoted) /* The next argument pointer has been moved to before the quoted region, so pretend we never saw the quoting "--", and give getopt another chance. If the user hasn't removed it, getopt will just process it again. */ parser->state.quoted = 0; if (parser->try_getopt && !parser->state.quoted) /* Give getopt a chance to parse this. */ { /* Put it back in OPTIND for getopt. */ parser->opt_data.optind = parser->state.next; /* Distinguish KEY_ERR from a real option. */ parser->opt_data.optopt = KEY_END; if (parser->state.flags & ARGP_LONG_ONLY) opt = _getopt_long_only_r (parser->state.argc, parser->state.argv, parser->short_opts, parser->long_opts, 0, &parser->opt_data); else opt = _getopt_long_r (parser->state.argc, parser->state.argv, parser->short_opts, parser->long_opts, 0, &parser->opt_data); /* And see what getopt did. */ parser->state.next = parser->opt_data.optind; if (opt == KEY_END) /* Getopt says there are no more options, so stop using getopt; we'll continue if necessary on our own. */ { parser->try_getopt = 0; if (parser->state.next > 1 && strcmp (parser->state.argv[parser->state.next - 1], QUOTE) == 0) /* Not only is this the end of the options, but it's a "quoted" region, which may have args that *look* like options, so we definitely shouldn't try to use getopt past here, whatever happens. */ parser->state.quoted = parser->state.next; } else if (opt == KEY_ERR && parser->opt_data.optopt != KEY_END) /* KEY_ERR can have the same value as a valid user short option, but in the case of a real error, getopt sets OPTOPT to the offending character, which can never be KEY_END. */ { *arg_ebadkey = 0; return EBADKEY; } } else opt = KEY_END; if (opt == KEY_END) { /* We're past what getopt considers the options. */ if (parser->state.next >= parser->state.argc || (parser->state.flags & ARGP_NO_ARGS)) /* Indicate that we're done. */ { *arg_ebadkey = 1; return EBADKEY; } else /* A non-option arg; simulate what getopt might have done. */ { opt = KEY_ARG; parser->opt_data.optarg = parser->state.argv[parser->state.next++]; } } if (opt == KEY_ARG) /* A non-option argument; try each parser in turn. */ err = parser_parse_arg (parser, parser->opt_data.optarg); else err = parser_parse_opt (parser, opt, parser->opt_data.optarg); if (err == EBADKEY) *arg_ebadkey = (opt == KEY_END || opt == KEY_ARG); return err; } /* Parse the options strings in ARGC & ARGV according to the argp in ARGP. FLAGS is one of the ARGP_ flags above. If END_INDEX is non-NULL, the index in ARGV of the first unparsed option is returned in it. If an unknown option is present, EINVAL is returned; if some parser routine returned a non-zero value, it is returned; otherwise 0 is returned. */ error_t __argp_parse (const struct argp *argp, int argc, char **argv, unsigned flags, int *end_index, void *input) { error_t err; struct parser parser; /* If true, then err == EBADKEY is a result of a non-option argument failing to be parsed (which in some cases isn't actually an error). */ int arg_ebadkey = 0; #ifndef _LIBC if (!(flags & ARGP_PARSE_ARGV0)) { #if HAVE_DECL_PROGRAM_INVOCATION_NAME if (!program_invocation_name) program_invocation_name = argv[0]; #endif #if HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME if (!program_invocation_short_name) program_invocation_short_name = __argp_base_name (argv[0]); #endif } #endif if (! (flags & ARGP_NO_HELP)) /* Add our own options. */ { struct argp_child *child = alloca (4 * sizeof (struct argp_child)); struct argp *top_argp = alloca (sizeof (struct argp)); /* TOP_ARGP has no options, it just serves to group the user & default argps. */ memset (top_argp, 0, sizeof (*top_argp)); top_argp->children = child; memset (child, 0, 4 * sizeof (struct argp_child)); if (argp) (child++)->argp = argp; (child++)->argp = &argp_default_argp; if (argp_program_version || argp_program_version_hook) (child++)->argp = &argp_version_argp; child->argp = 0; argp = top_argp; } /* Construct a parser for these arguments. */ err = parser_init (&parser, argp, argc, argv, flags, input); if (! err) /* Parse! */ { while (! err) err = parser_parse_next (&parser, &arg_ebadkey); err = parser_finalize (&parser, err, arg_ebadkey, end_index); } return err; } #ifdef weak_alias weak_alias (__argp_parse, argp_parse) #endif /* Return the input field for ARGP in the parser corresponding to STATE; used by the help routines. */ void * __argp_input (const struct argp *argp, const struct argp_state *state) { if (state) { struct group *group; struct parser *parser = state->pstate; for (group = parser->groups; group < parser->egroup; group++) if (group->argp == argp) return group->input; } return 0; } #ifdef weak_alias weak_alias (__argp_input, _argp_input) #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/argp-namefrob.h0000644000175000017500000001253313004436754017274 00000000000000/* Name frobnication for compiling argp outside of glibc Copyright (C) 1997-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #if !_LIBC /* This code is written for inclusion in gnu-libc, and uses names in the namespace reserved for libc. If we're not compiling in libc, define those names to be the normal ones instead. */ /* argp-parse functions */ #undef __argp_parse #define __argp_parse argp_parse #undef __option_is_end #define __option_is_end _option_is_end #undef __option_is_short #define __option_is_short _option_is_short #undef __argp_input #define __argp_input _argp_input /* argp-help functions */ #undef __argp_help #define __argp_help argp_help #undef __argp_error #define __argp_error argp_error #undef __argp_failure #define __argp_failure argp_failure #undef __argp_state_help #define __argp_state_help argp_state_help #undef __argp_usage #define __argp_usage argp_usage /* argp-fmtstream functions */ #undef __argp_make_fmtstream #define __argp_make_fmtstream argp_make_fmtstream #undef __argp_fmtstream_free #define __argp_fmtstream_free argp_fmtstream_free #undef __argp_fmtstream_putc #define __argp_fmtstream_putc argp_fmtstream_putc #undef __argp_fmtstream_puts #define __argp_fmtstream_puts argp_fmtstream_puts #undef __argp_fmtstream_write #define __argp_fmtstream_write argp_fmtstream_write #undef __argp_fmtstream_printf #define __argp_fmtstream_printf argp_fmtstream_printf #undef __argp_fmtstream_set_lmargin #define __argp_fmtstream_set_lmargin argp_fmtstream_set_lmargin #undef __argp_fmtstream_set_rmargin #define __argp_fmtstream_set_rmargin argp_fmtstream_set_rmargin #undef __argp_fmtstream_set_wmargin #define __argp_fmtstream_set_wmargin argp_fmtstream_set_wmargin #undef __argp_fmtstream_point #define __argp_fmtstream_point argp_fmtstream_point #undef __argp_fmtstream_update #define __argp_fmtstream_update _argp_fmtstream_update #undef __argp_fmtstream_ensure #define __argp_fmtstream_ensure _argp_fmtstream_ensure #undef __argp_fmtstream_lmargin #define __argp_fmtstream_lmargin argp_fmtstream_lmargin #undef __argp_fmtstream_rmargin #define __argp_fmtstream_rmargin argp_fmtstream_rmargin #undef __argp_fmtstream_wmargin #define __argp_fmtstream_wmargin argp_fmtstream_wmargin /* normal libc functions we call */ #undef __flockfile #define __flockfile flockfile #undef __funlockfile #define __funlockfile funlockfile #undef __mempcpy #define __mempcpy mempcpy #undef __sleep #define __sleep sleep #undef __strcasecmp #define __strcasecmp strcasecmp #undef __strchrnul #define __strchrnul strchrnul #undef __strerror_r #define __strerror_r strerror_r #undef __strndup #define __strndup strndup #undef __vsnprintf #define __vsnprintf vsnprintf #if defined(HAVE_DECL_CLEARERR_UNLOCKED) && !HAVE_DECL_CLEARERR_UNLOCKED # define clearerr_unlocked(x) clearerr (x) #endif #if defined(HAVE_DECL_FEOF_UNLOCKED) && !HAVE_DECL_FEOF_UNLOCKED # define feof_unlocked(x) feof (x) #endif #if defined(HAVE_DECL_FERROR_UNLOCKED) && !HAVE_DECL_FERROR_UNLOCKED # define ferror_unlocked(x) ferror (x) #endif #if defined(HAVE_DECL_FFLUSH_UNLOCKED) && !HAVE_DECL_FFLUSH_UNLOCKED # define fflush_unlocked(x) fflush (x) #endif #if defined(HAVE_DECL_FGETS_UNLOCKED) && !HAVE_DECL_FGETS_UNLOCKED # define fgets_unlocked(x,y,z) fgets (x,y,z) #endif #if defined(HAVE_DECL_FPUTC_UNLOCKED) && !HAVE_DECL_FPUTC_UNLOCKED # define fputc_unlocked(x,y) fputc (x,y) #endif #if defined(HAVE_DECL_FPUTS_UNLOCKED) && !HAVE_DECL_FPUTS_UNLOCKED # define fputs_unlocked(x,y) fputs (x,y) #endif #if defined(HAVE_DECL_FREAD_UNLOCKED) && !HAVE_DECL_FREAD_UNLOCKED # define fread_unlocked(w,x,y,z) fread (w,x,y,z) #endif #if defined(HAVE_DECL_FWRITE_UNLOCKED) && !HAVE_DECL_FWRITE_UNLOCKED # define fwrite_unlocked(w,x,y,z) fwrite (w,x,y,z) #endif #if defined(HAVE_DECL_GETC_UNLOCKED) && !HAVE_DECL_GETC_UNLOCKED # define getc_unlocked(x) getc (x) #endif #if defined(HAVE_DECL_GETCHAR_UNLOCKED) && !HAVE_DECL_GETCHAR_UNLOCKED # define getchar_unlocked() getchar () #endif #if defined(HAVE_DECL_PUTC_UNLOCKED) && !HAVE_DECL_PUTC_UNLOCKED # define putc_unlocked(x,y) putc (x,y) #endif #if defined(HAVE_DECL_PUTCHAR_UNLOCKED) && !HAVE_DECL_PUTCHAR_UNLOCKED # define putchar_unlocked(x) putchar (x) #endif #endif /* !_LIBC */ #ifndef __set_errno #define __set_errno(e) (errno = (e)) #endif #if defined GNULIB_ARGP_DISABLE_DIRNAME # define __argp_base_name(arg) arg #elif defined GNULIB_ARGP_EXTERN_BASENAME extern char *__argp_base_name (const char *arg); #else # include "dirname.h" # define __argp_base_name last_component #endif #if defined _LIBC || HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME # define __argp_short_program_name() (program_invocation_short_name) #else extern char *__argp_short_program_name (void); #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/argp-help.c0000644000175000017500000017212413004436754016431 00000000000000/* Hierarchical argument parsing help output Copyright (C) 1995-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _GNU_SOURCE # define _GNU_SOURCE 1 #endif #ifdef HAVE_CONFIG_H # include #endif #include #include #include #include #include #include #include #include #include #include #ifdef _LIBC # include <../libio/libioP.h> # include #endif #ifdef _LIBC # include # undef dgettext # define dgettext(domain, msgid) \ __dcgettext (domain, msgid, LC_MESSAGES) #else # include "gettext.h" #endif #include "argp.h" #include "argp-fmtstream.h" #include "argp-namefrob.h" #ifndef SIZE_MAX # define SIZE_MAX ((size_t) -1) #endif /* User-selectable (using an environment variable) formatting parameters. These may be specified in an environment variable called 'ARGP_HELP_FMT', with a contents like: VAR1=VAL1,VAR2=VAL2,BOOLVAR2,no-BOOLVAR2 Where VALn must be a positive integer. The list of variables is in the UPARAM_NAMES vector, below. */ /* Default parameters. */ #define DUP_ARGS 0 /* True if option argument can be duplicated. */ #define DUP_ARGS_NOTE 1 /* True to print a note about duplicate args. */ #define SHORT_OPT_COL 2 /* column in which short options start */ #define LONG_OPT_COL 6 /* column in which long options start */ #define DOC_OPT_COL 2 /* column in which doc options start */ #define OPT_DOC_COL 29 /* column in which option text starts */ #define HEADER_COL 1 /* column in which group headers are printed */ #define USAGE_INDENT 12 /* indentation of wrapped usage lines */ #define RMARGIN 79 /* right margin used for wrapping */ /* User-selectable (using an environment variable) formatting parameters. They must all be of type 'int' for the parsing code to work. */ struct uparams { /* If true, arguments for an option are shown with both short and long options, even when a given option has both, e.g. '-x ARG, --longx=ARG'. If false, then if an option has both, the argument is only shown with the long one, e.g., '-x, --longx=ARG', and a message indicating that this really means both is printed below the options. */ int dup_args; /* This is true if when DUP_ARGS is false, and some duplicate arguments have been suppressed, an explanatory message should be printed. */ int dup_args_note; /* Various output columns. */ int short_opt_col; /* column in which short options start */ int long_opt_col; /* column in which long options start */ int doc_opt_col; /* column in which doc options start */ int opt_doc_col; /* column in which option text starts */ int header_col; /* column in which group headers are printed */ int usage_indent; /* indentation of wrapped usage lines */ int rmargin; /* right margin used for wrapping */ int valid; /* True when the values in here are valid. */ }; /* This is a global variable, as user options are only ever read once. */ static struct uparams uparams = { DUP_ARGS, DUP_ARGS_NOTE, SHORT_OPT_COL, LONG_OPT_COL, DOC_OPT_COL, OPT_DOC_COL, HEADER_COL, USAGE_INDENT, RMARGIN }; /* A particular uparam, and what the user name is. */ struct uparam_name { const char name[14]; /* User name. */ bool is_bool; /* Whether it's 'boolean'. */ unsigned char uparams_offs; /* Location of the (int) field in UPARAMS. */ }; /* The name-field mappings we know about. */ static const struct uparam_name uparam_names[] = { { "dup-args", true, offsetof (struct uparams, dup_args) }, { "dup-args-note", true, offsetof (struct uparams, dup_args_note) }, { "short-opt-col", false, offsetof (struct uparams, short_opt_col) }, { "long-opt-col", false, offsetof (struct uparams, long_opt_col) }, { "doc-opt-col", false, offsetof (struct uparams, doc_opt_col) }, { "opt-doc-col", false, offsetof (struct uparams, opt_doc_col) }, { "header-col", false, offsetof (struct uparams, header_col) }, { "usage-indent", false, offsetof (struct uparams, usage_indent) }, { "rmargin", false, offsetof (struct uparams, rmargin) } }; #define nuparam_names (sizeof (uparam_names) / sizeof (uparam_names[0])) static void validate_uparams (const struct argp_state *state, struct uparams *upptr) { const struct uparam_name *up; for (up = uparam_names; up < uparam_names + nuparam_names; up++) { if (up->is_bool || up->uparams_offs == offsetof (struct uparams, rmargin)) continue; if (*(int *)((char *)upptr + up->uparams_offs) >= upptr->rmargin) { __argp_failure (state, 0, 0, dgettext (state->root_argp->argp_domain, "\ ARGP_HELP_FMT: %s value is less than or equal to %s"), "rmargin", up->name); return; } } uparams = *upptr; uparams.valid = 1; } /* Read user options from the environment, and fill in UPARAMS appropriately. */ static void fill_in_uparams (const struct argp_state *state) { const char *var = getenv ("ARGP_HELP_FMT"); struct uparams new_params = uparams; #define SKIPWS(p) do { while (isspace ((unsigned char) *p)) p++; } while (0); if (var) { /* Parse var. */ while (*var) { SKIPWS (var); if (isalpha ((unsigned char) *var)) { size_t var_len; const struct uparam_name *un; int unspec = 0, val = 0; const char *arg = var; while (isalnum ((unsigned char) *arg) || *arg == '-' || *arg == '_') arg++; var_len = arg - var; SKIPWS (arg); if (*arg == '\0' || *arg == ',') unspec = 1; else if (*arg == '=') { arg++; SKIPWS (arg); } if (unspec) { if (var[0] == 'n' && var[1] == 'o' && var[2] == '-') { val = 0; var += 3; var_len -= 3; } else val = 1; } else if (isdigit ((unsigned char) *arg)) { val = atoi (arg); while (isdigit ((unsigned char) *arg)) arg++; SKIPWS (arg); } for (un = uparam_names; un < uparam_names + nuparam_names; un++) if (strlen (un->name) == var_len && strncmp (var, un->name, var_len) == 0) { if (unspec && !un->is_bool) __argp_failure (state, 0, 0, dgettext (state == NULL ? NULL : state->root_argp->argp_domain, "\ %.*s: ARGP_HELP_FMT parameter requires a value"), (int) var_len, var); else *(int *)((char *)&new_params + un->uparams_offs) = val; break; } if (un == uparam_names + nuparam_names) __argp_failure (state, 0, 0, dgettext (state == NULL ? NULL : state->root_argp->argp_domain, "\ %.*s: Unknown ARGP_HELP_FMT parameter"), (int) var_len, var); var = arg; if (*var == ',') var++; } else if (*var) { __argp_failure (state, 0, 0, dgettext (state == NULL ? NULL : state->root_argp->argp_domain, "Garbage in ARGP_HELP_FMT: %s"), var); break; } } validate_uparams (state, &new_params); } } /* Returns true if OPT hasn't been marked invisible. Visibility only affects whether OPT is displayed or used in sorting, not option shadowing. */ #define ovisible(opt) (! ((opt)->flags & OPTION_HIDDEN)) /* Returns true if OPT is an alias for an earlier option. */ #define oalias(opt) ((opt)->flags & OPTION_ALIAS) /* Returns true if OPT is a documentation-only entry. */ #define odoc(opt) ((opt)->flags & OPTION_DOC) /* Returns true if OPT should not be translated */ #define onotrans(opt) ((opt)->flags & OPTION_NO_TRANS) /* Returns true if OPT is the end-of-list marker for a list of options. */ #define oend(opt) __option_is_end (opt) /* Returns true if OPT has a short option. */ #define oshort(opt) __option_is_short (opt) /* The help format for a particular option is like: -xARG, -yARG, --long1=ARG, --long2=ARG Documentation... Where ARG will be omitted if there's no argument, for this option, or will be surrounded by "[" and "]" appropriately if the argument is optional. The documentation string is word-wrapped appropriately, and if the list of options is long enough, it will be started on a separate line. If there are no short options for a given option, the first long option is indented slightly in a way that's supposed to make most long options appear to be in a separate column. For example, the following output (from ps): -p PID, --pid=PID List the process PID --pgrp=PGRP List processes in the process group PGRP -P, -x, --no-parent Include processes without parents -Q, --all-fields Don't elide unusable fields (normally if there's some reason ps can't print a field for any process, it's removed from the output entirely) -r, --reverse, --gratuitously-long-reverse-option Reverse the order of any sort --session[=SID] Add the processes from the session SID (which defaults to the sid of the current process) Here are some more options: -f ZOT, --foonly=ZOT Glork a foonly -z, --zaza Snit a zar -?, --help Give this help list --usage Give a short usage message -V, --version Print program version The struct argp_option array for the above could look like: { {"pid", 'p', "PID", 0, "List the process PID"}, {"pgrp", OPT_PGRP, "PGRP", 0, "List processes in the process group PGRP"}, {"no-parent", 'P', 0, 0, "Include processes without parents"}, {0, 'x', 0, OPTION_ALIAS}, {"all-fields",'Q', 0, 0, "Don't elide unusable fields (normally" " if there's some reason ps can't" " print a field for any process, it's" " removed from the output entirely)" }, {"reverse", 'r', 0, 0, "Reverse the order of any sort"}, {"gratuitously-long-reverse-option", 0, 0, OPTION_ALIAS}, {"session", OPT_SESS, "SID", OPTION_ARG_OPTIONAL, "Add the processes from the session" " SID (which defaults to the sid of" " the current process)" }, {0,0,0,0, "Here are some more options:"}, {"foonly", 'f', "ZOT", 0, "Glork a foonly"}, {"zaza", 'z', 0, 0, "Snit a zar"}, {0} } Note that the last three options are automatically supplied by argp_parse, unless you tell it not to with ARGP_NO_HELP. */ /* Returns true if CH occurs between BEG and END. */ static int find_char (char ch, char *beg, char *end) { while (beg < end) if (*beg == ch) return 1; else beg++; return 0; } struct hol_cluster; /* fwd decl */ struct hol_entry { /* First option. */ const struct argp_option *opt; /* Number of options (including aliases). */ unsigned num; /* A pointers into the HOL's short_options field, to the first short option letter for this entry. The order of the characters following this point corresponds to the order of options pointed to by OPT, and there are at most NUM. A short option recorded in an option following OPT is only valid if it occurs in the right place in SHORT_OPTIONS (otherwise it's probably been shadowed by some other entry). */ char *short_options; /* Entries are sorted by their group first, in the order: 1, 2, ..., n, 0, -m, ..., -2, -1 and then alphabetically within each group. The default is 0. */ int group; /* The cluster of options this entry belongs to, or 0 if none. */ struct hol_cluster *cluster; /* The argp from which this option came. */ const struct argp *argp; /* Position in the array */ unsigned ord; }; /* A cluster of entries to reflect the argp tree structure. */ struct hol_cluster { /* A descriptive header printed before options in this cluster. */ const char *header; /* Used to order clusters within the same group with the same parent, according to the order in which they occurred in the parent argp's child list. */ int index; /* How to sort this cluster with respect to options and other clusters at the same depth (clusters always follow options in the same group). */ int group; /* The cluster to which this cluster belongs, or 0 if it's at the base level. */ struct hol_cluster *parent; /* The argp from which this cluster is (eventually) derived. */ const struct argp *argp; /* The distance this cluster is from the root. */ int depth; /* Clusters in a given hol are kept in a linked list, to make freeing them possible. */ struct hol_cluster *next; }; /* A list of options for help. */ struct hol { /* An array of hol_entry's. */ struct hol_entry *entries; /* The number of entries in this hol. If this field is zero, the others are undefined. */ unsigned num_entries; /* A string containing all short options in this HOL. Each entry contains pointers into this string, so the order can't be messed with blindly. */ char *short_options; /* Clusters of entries in this hol. */ struct hol_cluster *clusters; }; /* Create a struct hol from the options in ARGP. CLUSTER is the hol_cluster in which these entries occur, or 0, if at the root. */ static struct hol * make_hol (const struct argp *argp, struct hol_cluster *cluster) { char *so; const struct argp_option *o; const struct argp_option *opts = argp->options; struct hol_entry *entry; unsigned num_short_options = 0; struct hol *hol = malloc (sizeof (struct hol)); assert (hol); hol->num_entries = 0; hol->clusters = 0; if (opts) { int cur_group = 0; /* The first option must not be an alias. */ assert (! oalias (opts)); /* Calculate the space needed. */ for (o = opts; ! oend (o); o++) { if (! oalias (o)) hol->num_entries++; if (oshort (o)) num_short_options++; /* This is an upper bound. */ } hol->entries = malloc (sizeof (struct hol_entry) * hol->num_entries); hol->short_options = malloc (num_short_options + 1); assert (hol->entries && hol->short_options); if (SIZE_MAX <= UINT_MAX) assert (hol->num_entries <= SIZE_MAX / sizeof (struct hol_entry)); /* Fill in the entries. */ so = hol->short_options; for (o = opts, entry = hol->entries; ! oend (o); entry++) { entry->opt = o; entry->num = 0; entry->short_options = so; entry->group = cur_group = o->group ? o->group : ((!o->name && !o->key) ? cur_group + 1 : cur_group); entry->cluster = cluster; entry->argp = argp; do { entry->num++; if (oshort (o) && ! find_char (o->key, hol->short_options, so)) /* O has a valid short option which hasn't already been used.*/ *so++ = o->key; o++; } while (! oend (o) && oalias (o)); } *so = '\0'; /* null terminated so we can find the length */ } return hol; } /* Add a new cluster to HOL, with the given GROUP and HEADER (taken from the associated argp child list entry), INDEX, and PARENT, and return a pointer to it. ARGP is the argp that this cluster results from. */ static struct hol_cluster * hol_add_cluster (struct hol *hol, int group, const char *header, int index, struct hol_cluster *parent, const struct argp *argp) { struct hol_cluster *cl = malloc (sizeof (struct hol_cluster)); if (cl) { cl->group = group; cl->header = header; cl->index = index; cl->parent = parent; cl->argp = argp; cl->depth = parent ? parent->depth + 1 : 0; cl->next = hol->clusters; hol->clusters = cl; } return cl; } /* Free HOL and any resources it uses. */ static void hol_free (struct hol *hol) { struct hol_cluster *cl = hol->clusters; while (cl) { struct hol_cluster *next = cl->next; free (cl); cl = next; } if (hol->num_entries > 0) { free (hol->entries); free (hol->short_options); } free (hol); } static int hol_entry_short_iterate (const struct hol_entry *entry, int (*func)(const struct argp_option *opt, const struct argp_option *real, const char *domain, void *cookie), const char *domain, void *cookie) { unsigned nopts; int val = 0; const struct argp_option *opt, *real = entry->opt; char *so = entry->short_options; for (opt = real, nopts = entry->num; nopts > 0 && !val; opt++, nopts--) if (oshort (opt) && *so == opt->key) { if (!oalias (opt)) real = opt; if (ovisible (opt)) val = (*func)(opt, real, domain, cookie); so++; } return val; } static inline int #if __GNUC__ >= 3 __attribute__ ((always_inline)) #endif hol_entry_long_iterate (const struct hol_entry *entry, int (*func)(const struct argp_option *opt, const struct argp_option *real, const char *domain, void *cookie), const char *domain, void *cookie) { unsigned nopts; int val = 0; const struct argp_option *opt, *real = entry->opt; for (opt = real, nopts = entry->num; nopts > 0 && !val; opt++, nopts--) if (opt->name) { if (!oalias (opt)) real = opt; if (ovisible (opt)) val = (*func)(opt, real, domain, cookie); } return val; } /* Iterator that returns true for the first short option. */ static int until_short (const struct argp_option *opt, const struct argp_option *real, const char *domain, void *cookie) { return oshort (opt) ? opt->key : 0; } /* Returns the first valid short option in ENTRY, or 0 if there is none. */ static char hol_entry_first_short (const struct hol_entry *entry) { return hol_entry_short_iterate (entry, until_short, entry->argp->argp_domain, 0); } /* Returns the first valid long option in ENTRY, or 0 if there is none. */ static const char * hol_entry_first_long (const struct hol_entry *entry) { const struct argp_option *opt; unsigned num; for (opt = entry->opt, num = entry->num; num > 0; opt++, num--) if (opt->name && ovisible (opt)) return opt->name; return 0; } /* Returns the entry in HOL with the long option name NAME, or 0 if there is none. */ static struct hol_entry * hol_find_entry (struct hol *hol, const char *name) { struct hol_entry *entry = hol->entries; unsigned num_entries = hol->num_entries; while (num_entries-- > 0) { const struct argp_option *opt = entry->opt; unsigned num_opts = entry->num; while (num_opts-- > 0) if (opt->name && ovisible (opt) && strcmp (opt->name, name) == 0) return entry; else opt++; entry++; } return 0; } /* If an entry with the long option NAME occurs in HOL, set its special sort position to GROUP. */ static void hol_set_group (struct hol *hol, const char *name, int group) { struct hol_entry *entry = hol_find_entry (hol, name); if (entry) entry->group = group; } /* Order by group: 0, 1, 2, ..., n, -m, ..., -2, -1. EQ is what to return if GROUP1 and GROUP2 are the same. */ static int group_cmp (int group1, int group2, int eq) { if (group1 == group2) return eq; else if ((group1 < 0 && group2 < 0) || (group1 >= 0 && group2 >= 0)) return group1 - group2; else return group2 - group1; } /* Compare clusters CL1 & CL2 by the order that they should appear in output. */ static int hol_cluster_cmp (const struct hol_cluster *cl1, const struct hol_cluster *cl2) { /* If one cluster is deeper than the other, use its ancestor at the same level, so that finding the common ancestor is straightforward. */ while (cl1->depth > cl2->depth) cl1 = cl1->parent; while (cl2->depth > cl1->depth) cl2 = cl2->parent; /* Now reduce both clusters to their ancestors at the point where both have a common parent; these can be directly compared. */ while (cl1->parent != cl2->parent) cl1 = cl1->parent, cl2 = cl2->parent; return group_cmp (cl1->group, cl2->group, cl2->index - cl1->index); } /* Return the ancestor of CL that's just below the root (i.e., has a parent of 0). */ static struct hol_cluster * hol_cluster_base (struct hol_cluster *cl) { while (cl->parent) cl = cl->parent; return cl; } /* Return true if CL1 is a child of CL2. */ static int hol_cluster_is_child (const struct hol_cluster *cl1, const struct hol_cluster *cl2) { while (cl1 && cl1 != cl2) cl1 = cl1->parent; return cl1 == cl2; } /* Given the name of an OPTION_DOC option, modifies NAME to start at the tail that should be used for comparisons, and returns true iff it should be treated as a non-option. */ static int canon_doc_option (const char **name) { int non_opt; /* Skip initial whitespace. */ while (isspace (**name)) (*name)++; /* Decide whether this looks like an option (leading '-') or not. */ non_opt = (**name != '-'); /* Skip until part of name used for sorting. */ while (**name && !isalnum (**name)) (*name)++; return non_opt; } #define HOL_ENTRY_PTRCMP(a,b) ((a)->ord < (b)->ord ? -1 : 1) /* Order ENTRY1 & ENTRY2 by the order which they should appear in a help listing. */ static int hol_entry_cmp (const struct hol_entry *entry1, const struct hol_entry *entry2) { /* The group numbers by which the entries should be ordered; if either is in a cluster, then this is just the group within the cluster. */ int group1 = entry1->group, group2 = entry2->group; if (entry1->cluster != entry2->cluster) { /* The entries are not within the same cluster, so we can't compare them directly, we have to use the appropriate clustering level too. */ if (! entry1->cluster) /* ENTRY1 is at the 'base level', not in a cluster, so we have to compare it's group number with that of the base cluster in which ENTRY2 resides. Note that if they're in the same group, the clustered option always comes last. */ return group_cmp (group1, hol_cluster_base (entry2->cluster)->group, -1); else if (! entry2->cluster) /* Likewise, but ENTRY2's not in a cluster. */ return group_cmp (hol_cluster_base (entry1->cluster)->group, group2, 1); else /* Both entries are in clusters, we can just compare the clusters. */ return hol_cluster_cmp (entry1->cluster, entry2->cluster); } else if (group1 == group2) /* The entries are both in the same cluster and group, so compare them alphabetically. */ { int short1 = hol_entry_first_short (entry1); int short2 = hol_entry_first_short (entry2); int doc1 = odoc (entry1->opt); int doc2 = odoc (entry2->opt); const char *long1 = hol_entry_first_long (entry1); const char *long2 = hol_entry_first_long (entry2); if (doc1) doc1 = long1 != NULL && canon_doc_option (&long1); if (doc2) doc2 = long2 != NULL && canon_doc_option (&long2); if (doc1 != doc2) /* 'documentation' options always follow normal options (or documentation options that *look* like normal options). */ return doc1 - doc2; else if (!short1 && !short2 && long1 && long2) /* Only long options. */ return __strcasecmp (long1, long2); else /* Compare short/short, long/short, short/long, using the first character of long options. Entries without *any* valid options (such as options with OPTION_HIDDEN set) will be put first, but as they're not displayed, it doesn't matter where they are. */ { char first1 = short1 ? short1 : long1 ? *long1 : 0; char first2 = short2 ? short2 : long2 ? *long2 : 0; #ifdef _tolower int lower_cmp = _tolower (first1) - _tolower (first2); #else int lower_cmp = tolower (first1) - tolower (first2); #endif /* Compare ignoring case, except when the options are both the same letter, in which case lower-case always comes first. */ return lower_cmp ? lower_cmp : first2 - first1; } } else /* Within the same cluster, but not the same group, so just compare groups. */ return group_cmp (group1, group2, 0); } /* Version of hol_entry_cmp with correct signature for qsort. */ static int hol_entry_qcmp (const void *entry1_v, const void *entry2_v) { return hol_entry_cmp (entry1_v, entry2_v); } /* Sort HOL by group and alphabetically by option name (with short options taking precedence over long). Since the sorting is for display purposes only, the shadowing of options isn't effected. */ static void hol_sort (struct hol *hol) { if (hol->num_entries > 0) { unsigned i; struct hol_entry *e; for (i = 0, e = hol->entries; i < hol->num_entries; i++, e++) e->ord = i; qsort (hol->entries, hol->num_entries, sizeof (struct hol_entry), hol_entry_qcmp); } } /* Append MORE to HOL, destroying MORE in the process. Options in HOL shadow any in MORE with the same name. */ static void hol_append (struct hol *hol, struct hol *more) { struct hol_cluster **cl_end = &hol->clusters; /* Steal MORE's cluster list, and add it to the end of HOL's. */ while (*cl_end) cl_end = &(*cl_end)->next; *cl_end = more->clusters; more->clusters = 0; /* Merge entries. */ if (more->num_entries > 0) { if (hol->num_entries == 0) { hol->num_entries = more->num_entries; hol->entries = more->entries; hol->short_options = more->short_options; more->num_entries = 0; /* Mark MORE's fields as invalid. */ } else /* Append the entries in MORE to those in HOL, taking care to only add non-shadowed SHORT_OPTIONS values. */ { unsigned left; char *so, *more_so; struct hol_entry *e; unsigned num_entries = hol->num_entries + more->num_entries; struct hol_entry *entries = malloc (num_entries * sizeof (struct hol_entry)); unsigned hol_so_len = strlen (hol->short_options); char *short_options = malloc (hol_so_len + strlen (more->short_options) + 1); assert (entries && short_options); if (SIZE_MAX <= UINT_MAX) assert (num_entries <= SIZE_MAX / sizeof (struct hol_entry)); __mempcpy (__mempcpy (entries, hol->entries, hol->num_entries * sizeof (struct hol_entry)), more->entries, more->num_entries * sizeof (struct hol_entry)); __mempcpy (short_options, hol->short_options, hol_so_len); /* Fix up the short options pointers from HOL. */ for (e = entries, left = hol->num_entries; left > 0; e++, left--) e->short_options += (short_options - hol->short_options); /* Now add the short options from MORE, fixing up its entries too. */ so = short_options + hol_so_len; more_so = more->short_options; for (left = more->num_entries; left > 0; e++, left--) { int opts_left; const struct argp_option *opt; e->short_options = so; for (opts_left = e->num, opt = e->opt; opts_left; opt++, opts_left--) { int ch = *more_so; if (oshort (opt) && ch == opt->key) /* The next short option in MORE_SO, CH, is from OPT. */ { if (! find_char (ch, short_options, short_options + hol_so_len)) /* The short option CH isn't shadowed by HOL's options, so add it to the sum. */ *so++ = ch; more_so++; } } } *so = '\0'; free (hol->entries); free (hol->short_options); hol->entries = entries; hol->num_entries = num_entries; hol->short_options = short_options; } } hol_free (more); } /* Inserts enough spaces to make sure STREAM is at column COL. */ static void indent_to (argp_fmtstream_t stream, unsigned col) { int needed = col - __argp_fmtstream_point (stream); while (needed-- > 0) __argp_fmtstream_putc (stream, ' '); } /* Output to STREAM either a space, or a newline if there isn't room for at least ENSURE characters before the right margin. */ static void space (argp_fmtstream_t stream, size_t ensure) { if (__argp_fmtstream_point (stream) + ensure >= __argp_fmtstream_rmargin (stream)) __argp_fmtstream_putc (stream, '\n'); else __argp_fmtstream_putc (stream, ' '); } /* If the option REAL has an argument, we print it in using the printf format REQ_FMT or OPT_FMT depending on whether it's a required or optional argument. */ static void arg (const struct argp_option *real, const char *req_fmt, const char *opt_fmt, const char *domain, argp_fmtstream_t stream) { if (real->arg) { if (real->flags & OPTION_ARG_OPTIONAL) __argp_fmtstream_printf (stream, opt_fmt, dgettext (domain, real->arg)); else __argp_fmtstream_printf (stream, req_fmt, dgettext (domain, real->arg)); } } /* Helper functions for hol_entry_help. */ /* State used during the execution of hol_help. */ struct hol_help_state { /* PREV_ENTRY should contain the previous entry printed, or 0. */ struct hol_entry *prev_entry; /* If an entry is in a different group from the previous one, and SEP_GROUPS is true, then a blank line will be printed before any output. */ int sep_groups; /* True if a duplicate option argument was suppressed (only ever set if UPARAMS.dup_args is false). */ int suppressed_dup_arg; }; /* Some state used while printing a help entry (used to communicate with helper functions). See the doc for hol_entry_help for more info, as most of the fields are copied from its arguments. */ struct pentry_state { const struct hol_entry *entry; argp_fmtstream_t stream; struct hol_help_state *hhstate; /* True if nothing's been printed so far. */ int first; /* If non-zero, the state that was used to print this help. */ const struct argp_state *state; }; /* If a user doc filter should be applied to DOC, do so. */ static const char * filter_doc (const char *doc, int key, const struct argp *argp, const struct argp_state *state) { if (argp && argp->help_filter) /* We must apply a user filter to this output. */ { void *input = __argp_input (argp, state); return (*argp->help_filter) (key, doc, input); } else /* No filter. */ return doc; } /* Prints STR as a header line, with the margin lines set appropriately, and notes the fact that groups should be separated with a blank line. ARGP is the argp that should dictate any user doc filtering to take place. Note that the previous wrap margin isn't restored, but the left margin is reset to 0. */ static void print_header (const char *str, const struct argp *argp, struct pentry_state *pest) { const char *tstr = dgettext (argp->argp_domain, str); const char *fstr = filter_doc (tstr, ARGP_KEY_HELP_HEADER, argp, pest->state); if (fstr) { if (*fstr) { if (pest->hhstate->prev_entry) /* Precede with a blank line. */ __argp_fmtstream_putc (pest->stream, '\n'); indent_to (pest->stream, uparams.header_col); __argp_fmtstream_set_lmargin (pest->stream, uparams.header_col); __argp_fmtstream_set_wmargin (pest->stream, uparams.header_col); __argp_fmtstream_puts (pest->stream, fstr); __argp_fmtstream_set_lmargin (pest->stream, 0); __argp_fmtstream_putc (pest->stream, '\n'); } pest->hhstate->sep_groups = 1; /* Separate subsequent groups. */ } if (fstr != tstr) free ((char *) fstr); } /* Inserts a comma if this isn't the first item on the line, and then makes sure we're at least to column COL. If this *is* the first item on a line, prints any pending whitespace/headers that should precede this line. Also clears FIRST. */ static void comma (unsigned col, struct pentry_state *pest) { if (pest->first) { const struct hol_entry *pe = pest->hhstate->prev_entry; const struct hol_cluster *cl = pest->entry->cluster; if (pest->hhstate->sep_groups && pe && pest->entry->group != pe->group) __argp_fmtstream_putc (pest->stream, '\n'); if (cl && cl->header && *cl->header && (!pe || (pe->cluster != cl && !hol_cluster_is_child (pe->cluster, cl)))) /* If we're changing clusters, then this must be the start of the ENTRY's cluster unless that is an ancestor of the previous one (in which case we had just popped into a sub-cluster for a bit). If so, then print the cluster's header line. */ { int old_wm = __argp_fmtstream_wmargin (pest->stream); print_header (cl->header, cl->argp, pest); __argp_fmtstream_set_wmargin (pest->stream, old_wm); } pest->first = 0; } else __argp_fmtstream_puts (pest->stream, ", "); indent_to (pest->stream, col); } /* Print help for ENTRY to STREAM. */ static void hol_entry_help (struct hol_entry *entry, const struct argp_state *state, argp_fmtstream_t stream, struct hol_help_state *hhstate) { unsigned num; const struct argp_option *real = entry->opt, *opt; char *so = entry->short_options; int have_long_opt = 0; /* We have any long options. */ /* Saved margins. */ int old_lm = __argp_fmtstream_set_lmargin (stream, 0); int old_wm = __argp_fmtstream_wmargin (stream); /* PEST is a state block holding some of our variables that we'd like to share with helper functions. */ struct pentry_state pest = { entry, stream, hhstate, 1, state }; if (! odoc (real)) for (opt = real, num = entry->num; num > 0; opt++, num--) if (opt->name && ovisible (opt)) { have_long_opt = 1; break; } /* First emit short options. */ __argp_fmtstream_set_wmargin (stream, uparams.short_opt_col); /* For truly bizarre cases. */ for (opt = real, num = entry->num; num > 0; opt++, num--) if (oshort (opt) && opt->key == *so) /* OPT has a valid (non shadowed) short option. */ { if (ovisible (opt)) { comma (uparams.short_opt_col, &pest); __argp_fmtstream_putc (stream, '-'); __argp_fmtstream_putc (stream, *so); if (!have_long_opt || uparams.dup_args) arg (real, " %s", "[%s]", state == NULL ? NULL : state->root_argp->argp_domain, stream); else if (real->arg) hhstate->suppressed_dup_arg = 1; } so++; } /* Now, long options. */ if (odoc (real)) /* A "documentation" option. */ { __argp_fmtstream_set_wmargin (stream, uparams.doc_opt_col); for (opt = real, num = entry->num; num > 0; opt++, num--) if (opt->name && ovisible (opt)) { comma (uparams.doc_opt_col, &pest); /* Calling dgettext here isn't quite right, since sorting will have been done on the original; but documentation options should be pretty rare anyway... */ __argp_fmtstream_puts (stream, dgettext (state == NULL ? NULL : state->root_argp->argp_domain, opt->name)); } } else /* A real long option. */ { __argp_fmtstream_set_wmargin (stream, uparams.long_opt_col); for (opt = real, num = entry->num; num > 0; opt++, num--) if (opt->name && ovisible (opt)) { comma (uparams.long_opt_col, &pest); __argp_fmtstream_printf (stream, "--%s", opt->name); arg (real, "=%s", "[=%s]", state == NULL ? NULL : state->root_argp->argp_domain, stream); } } /* Next, documentation strings. */ __argp_fmtstream_set_lmargin (stream, 0); if (pest.first) { /* Didn't print any switches, what's up? */ if (!oshort (real) && !real->name) /* This is a group header, print it nicely. */ print_header (real->doc, entry->argp, &pest); else /* Just a totally shadowed option or null header; print nothing. */ goto cleanup; /* Just return, after cleaning up. */ } else { const char *tstr = real->doc ? dgettext (state == NULL ? NULL : state->root_argp->argp_domain, real->doc) : 0; const char *fstr = filter_doc (tstr, real->key, entry->argp, state); if (fstr && *fstr) { unsigned int col = __argp_fmtstream_point (stream); __argp_fmtstream_set_lmargin (stream, uparams.opt_doc_col); __argp_fmtstream_set_wmargin (stream, uparams.opt_doc_col); if (col > (unsigned int) (uparams.opt_doc_col + 3)) __argp_fmtstream_putc (stream, '\n'); else if (col >= (unsigned int) uparams.opt_doc_col) __argp_fmtstream_puts (stream, " "); else indent_to (stream, uparams.opt_doc_col); __argp_fmtstream_puts (stream, fstr); } if (fstr && fstr != tstr) free ((char *) fstr); /* Reset the left margin. */ __argp_fmtstream_set_lmargin (stream, 0); __argp_fmtstream_putc (stream, '\n'); } hhstate->prev_entry = entry; cleanup: __argp_fmtstream_set_lmargin (stream, old_lm); __argp_fmtstream_set_wmargin (stream, old_wm); } /* Output a long help message about the options in HOL to STREAM. */ static void hol_help (struct hol *hol, const struct argp_state *state, argp_fmtstream_t stream) { unsigned num; struct hol_entry *entry; struct hol_help_state hhstate = { 0, 0, 0 }; for (entry = hol->entries, num = hol->num_entries; num > 0; entry++, num--) hol_entry_help (entry, state, stream, &hhstate); if (hhstate.suppressed_dup_arg && uparams.dup_args_note) { const char *tstr = dgettext (state == NULL ? NULL : state->root_argp->argp_domain, "\ Mandatory or optional arguments to long options are also mandatory or \ optional for any corresponding short options."); const char *fstr = filter_doc (tstr, ARGP_KEY_HELP_DUP_ARGS_NOTE, state ? state->root_argp : 0, state); if (fstr && *fstr) { __argp_fmtstream_putc (stream, '\n'); __argp_fmtstream_puts (stream, fstr); __argp_fmtstream_putc (stream, '\n'); } if (fstr && fstr != tstr) free ((char *) fstr); } } /* Helper functions for hol_usage. */ /* If OPT is a short option without an arg, append its key to the string pointer pointer to by COOKIE, and advance the pointer. */ static int add_argless_short_opt (const struct argp_option *opt, const struct argp_option *real, const char *domain, void *cookie) { char **snao_end = cookie; if (!(opt->arg || real->arg) && !((opt->flags | real->flags) & OPTION_NO_USAGE)) *(*snao_end)++ = opt->key; return 0; } /* If OPT is a short option with an arg, output a usage entry for it to the stream pointed at by COOKIE. */ static int usage_argful_short_opt (const struct argp_option *opt, const struct argp_option *real, const char *domain, void *cookie) { argp_fmtstream_t stream = cookie; const char *arg = opt->arg; int flags = opt->flags | real->flags; if (! arg) arg = real->arg; if (arg && !(flags & OPTION_NO_USAGE)) { arg = dgettext (domain, arg); if (flags & OPTION_ARG_OPTIONAL) __argp_fmtstream_printf (stream, " [-%c[%s]]", opt->key, arg); else { /* Manually do line wrapping so that it (probably) won't get wrapped at the embedded space. */ space (stream, 6 + strlen (arg)); __argp_fmtstream_printf (stream, "[-%c %s]", opt->key, arg); } } return 0; } /* Output a usage entry for the long option opt to the stream pointed at by COOKIE. */ static int usage_long_opt (const struct argp_option *opt, const struct argp_option *real, const char *domain, void *cookie) { argp_fmtstream_t stream = cookie; const char *arg = opt->arg; int flags = opt->flags | real->flags; if (! arg) arg = real->arg; if (! (flags & OPTION_NO_USAGE)) { if (arg) { arg = dgettext (domain, arg); if (flags & OPTION_ARG_OPTIONAL) __argp_fmtstream_printf (stream, " [--%s[=%s]]", opt->name, arg); else __argp_fmtstream_printf (stream, " [--%s=%s]", opt->name, arg); } else __argp_fmtstream_printf (stream, " [--%s]", opt->name); } return 0; } /* Print a short usage description for the arguments in HOL to STREAM. */ static void hol_usage (struct hol *hol, argp_fmtstream_t stream) { if (hol->num_entries > 0) { unsigned nentries; struct hol_entry *entry; char *short_no_arg_opts = alloca (strlen (hol->short_options) + 1); char *snao_end = short_no_arg_opts; /* First we put a list of short options without arguments. */ for (entry = hol->entries, nentries = hol->num_entries ; nentries > 0 ; entry++, nentries--) hol_entry_short_iterate (entry, add_argless_short_opt, entry->argp->argp_domain, &snao_end); if (snao_end > short_no_arg_opts) { *snao_end++ = 0; __argp_fmtstream_printf (stream, " [-%s]", short_no_arg_opts); } /* Now a list of short options *with* arguments. */ for (entry = hol->entries, nentries = hol->num_entries ; nentries > 0 ; entry++, nentries--) hol_entry_short_iterate (entry, usage_argful_short_opt, entry->argp->argp_domain, stream); /* Finally, a list of long options (whew!). */ for (entry = hol->entries, nentries = hol->num_entries ; nentries > 0 ; entry++, nentries--) hol_entry_long_iterate (entry, usage_long_opt, entry->argp->argp_domain, stream); } } /* Make a HOL containing all levels of options in ARGP. CLUSTER is the cluster in which ARGP's entries should be clustered, or 0. */ static struct hol * argp_hol (const struct argp *argp, struct hol_cluster *cluster) { const struct argp_child *child = argp->children; struct hol *hol = make_hol (argp, cluster); if (child) while (child->argp) { struct hol_cluster *child_cluster = ((child->group || child->header) /* Put CHILD->argp within its own cluster. */ ? hol_add_cluster (hol, child->group, child->header, child - argp->children, cluster, argp) /* Just merge it into the parent's cluster. */ : cluster); hol_append (hol, argp_hol (child->argp, child_cluster)) ; child++; } return hol; } /* Calculate how many different levels with alternative args strings exist in ARGP. */ static size_t argp_args_levels (const struct argp *argp) { size_t levels = 0; const struct argp_child *child = argp->children; if (argp->args_doc && strchr (argp->args_doc, '\n')) levels++; if (child) while (child->argp) levels += argp_args_levels ((child++)->argp); return levels; } /* Print all the non-option args documented in ARGP to STREAM. Any output is preceded by a space. LEVELS is a pointer to a byte vector the length returned by argp_args_levels; it should be initialized to zero, and updated by this routine for the next call if ADVANCE is true. True is returned as long as there are more patterns to output. */ static int argp_args_usage (const struct argp *argp, const struct argp_state *state, char **levels, int advance, argp_fmtstream_t stream) { char *our_level = *levels; int multiple = 0; const struct argp_child *child = argp->children; const char *tdoc = dgettext (argp->argp_domain, argp->args_doc), *nl = 0; const char *fdoc = filter_doc (tdoc, ARGP_KEY_HELP_ARGS_DOC, argp, state); if (fdoc) { const char *cp = fdoc; nl = __strchrnul (cp, '\n'); if (*nl != '\0') /* This is a 'multi-level' args doc; advance to the correct position as determined by our state in LEVELS, and update LEVELS. */ { int i; multiple = 1; for (i = 0; i < *our_level; i++) cp = nl + 1, nl = __strchrnul (cp, '\n'); (*levels)++; } /* Manually do line wrapping so that it (probably) won't get wrapped at any embedded spaces. */ space (stream, 1 + nl - cp); __argp_fmtstream_write (stream, cp, nl - cp); } if (fdoc && fdoc != tdoc) free ((char *)fdoc); /* Free user's modified doc string. */ if (child) while (child->argp) advance = !argp_args_usage ((child++)->argp, state, levels, advance, stream); if (advance && multiple) { /* Need to increment our level. */ if (*nl) /* There's more we can do here. */ { (*our_level)++; advance = 0; /* Our parent shouldn't advance also. */ } else if (*our_level > 0) /* We had multiple levels, but used them up; reset to zero. */ *our_level = 0; } return !advance; } /* Print the documentation for ARGP to STREAM; if POST is false, then everything preceeding a '\v' character in the documentation strings (or the whole string, for those with none) is printed, otherwise, everything following the '\v' character (nothing for strings without). Each separate bit of documentation is separated a blank line, and if PRE_BLANK is true, then the first is as well. If FIRST_ONLY is true, only the first occurrence is output. Returns true if anything was output. */ static int argp_doc (const struct argp *argp, const struct argp_state *state, int post, int pre_blank, int first_only, argp_fmtstream_t stream) { const char *text; const char *inp_text; void *input = 0; int anything = 0; size_t inp_text_limit = 0; const char *doc = dgettext (argp->argp_domain, argp->doc); const struct argp_child *child = argp->children; if (doc) { char *vt = strchr (doc, '\v'); inp_text = post ? (vt ? vt + 1 : 0) : doc; inp_text_limit = (!post && vt) ? (vt - doc) : 0; } else inp_text = 0; if (argp->help_filter) /* We have to filter the doc strings. */ { if (inp_text_limit) /* Copy INP_TEXT so that it's nul-terminated. */ inp_text = __strndup (inp_text, inp_text_limit); input = __argp_input (argp, state); text = (*argp->help_filter) (post ? ARGP_KEY_HELP_POST_DOC : ARGP_KEY_HELP_PRE_DOC, inp_text, input); } else text = (const char *) inp_text; if (text) { if (pre_blank) __argp_fmtstream_putc (stream, '\n'); if (text == inp_text && inp_text_limit) __argp_fmtstream_write (stream, inp_text, inp_text_limit); else __argp_fmtstream_puts (stream, text); if (__argp_fmtstream_point (stream) > __argp_fmtstream_lmargin (stream)) __argp_fmtstream_putc (stream, '\n'); anything = 1; } if (text && text != inp_text) free ((char *) text); /* Free TEXT returned from the help filter. */ if (inp_text && inp_text_limit && argp->help_filter) free ((char *) inp_text); /* We copied INP_TEXT, so free it now. */ if (post && argp->help_filter) /* Now see if we have to output a ARGP_KEY_HELP_EXTRA text. */ { text = (*argp->help_filter) (ARGP_KEY_HELP_EXTRA, 0, input); if (text) { if (anything || pre_blank) __argp_fmtstream_putc (stream, '\n'); __argp_fmtstream_puts (stream, text); free ((char *) text); if (__argp_fmtstream_point (stream) > __argp_fmtstream_lmargin (stream)) __argp_fmtstream_putc (stream, '\n'); anything = 1; } } if (child) while (child->argp && !(first_only && anything)) anything |= argp_doc ((child++)->argp, state, post, anything || pre_blank, first_only, stream); return anything; } /* Output a usage message for ARGP to STREAM. If called from argp_state_help, STATE is the relevent parsing state. FLAGS are from the set ARGP_HELP_*. NAME is what to use wherever a 'program name' is needed. */ static void _help (const struct argp *argp, const struct argp_state *state, FILE *stream, unsigned flags, char *name) { int anything = 0; /* Whether we've output anything. */ struct hol *hol = 0; argp_fmtstream_t fs; if (! stream) return; #if _LIBC || (HAVE_FLOCKFILE && HAVE_FUNLOCKFILE) __flockfile (stream); #endif if (! uparams.valid) fill_in_uparams (state); fs = __argp_make_fmtstream (stream, 0, uparams.rmargin, 0); if (! fs) { #if _LIBC || (HAVE_FLOCKFILE && HAVE_FUNLOCKFILE) __funlockfile (stream); #endif return; } if (flags & (ARGP_HELP_USAGE | ARGP_HELP_SHORT_USAGE | ARGP_HELP_LONG)) { hol = argp_hol (argp, 0); /* If present, these options always come last. */ hol_set_group (hol, "help", -1); hol_set_group (hol, "version", -1); hol_sort (hol); } if (flags & (ARGP_HELP_USAGE | ARGP_HELP_SHORT_USAGE)) /* Print a short "Usage:" message. */ { int first_pattern = 1, more_patterns; size_t num_pattern_levels = argp_args_levels (argp); char *pattern_levels = alloca (num_pattern_levels); memset (pattern_levels, 0, num_pattern_levels); do { int old_lm; int old_wm = __argp_fmtstream_set_wmargin (fs, uparams.usage_indent); char *levels = pattern_levels; if (first_pattern) __argp_fmtstream_printf (fs, "%s %s", dgettext (argp->argp_domain, "Usage:"), name); else __argp_fmtstream_printf (fs, "%s %s", dgettext (argp->argp_domain, " or: "), name); /* We set the lmargin as well as the wmargin, because hol_usage manually wraps options with newline to avoid annoying breaks. */ old_lm = __argp_fmtstream_set_lmargin (fs, uparams.usage_indent); if (flags & ARGP_HELP_SHORT_USAGE) /* Just show where the options go. */ { if (hol->num_entries > 0) __argp_fmtstream_puts (fs, dgettext (argp->argp_domain, " [OPTION...]")); } else /* Actually print the options. */ { hol_usage (hol, fs); flags |= ARGP_HELP_SHORT_USAGE; /* But only do so once. */ } more_patterns = argp_args_usage (argp, state, &levels, 1, fs); __argp_fmtstream_set_wmargin (fs, old_wm); __argp_fmtstream_set_lmargin (fs, old_lm); __argp_fmtstream_putc (fs, '\n'); anything = 1; first_pattern = 0; } while (more_patterns); } if (flags & ARGP_HELP_PRE_DOC) anything |= argp_doc (argp, state, 0, 0, 1, fs); if (flags & ARGP_HELP_SEE) { __argp_fmtstream_printf (fs, dgettext (argp->argp_domain, "\ Try '%s --help' or '%s --usage' for more information.\n"), name, name); anything = 1; } if (flags & ARGP_HELP_LONG) /* Print a long, detailed help message. */ { /* Print info about all the options. */ if (hol->num_entries > 0) { if (anything) __argp_fmtstream_putc (fs, '\n'); hol_help (hol, state, fs); anything = 1; } } if (flags & ARGP_HELP_POST_DOC) /* Print any documentation strings at the end. */ anything |= argp_doc (argp, state, 1, anything, 0, fs); if ((flags & ARGP_HELP_BUG_ADDR) && argp_program_bug_address) { if (anything) __argp_fmtstream_putc (fs, '\n'); __argp_fmtstream_printf (fs, dgettext (argp->argp_domain, "Report bugs to %s.\n"), argp_program_bug_address); anything = 1; } #if _LIBC || (HAVE_FLOCKFILE && HAVE_FUNLOCKFILE) __funlockfile (stream); #endif if (hol) hol_free (hol); __argp_fmtstream_free (fs); } /* Output a usage message for ARGP to STREAM. FLAGS are from the set ARGP_HELP_*. NAME is what to use wherever a 'program name' is needed. */ void __argp_help (const struct argp *argp, FILE *stream, unsigned flags, char *name) { _help (argp, 0, stream, flags, name); } #ifdef weak_alias weak_alias (__argp_help, argp_help) #endif #if ! (defined _LIBC || HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME) char * __argp_short_program_name (void) { # if HAVE_DECL_PROGRAM_INVOCATION_NAME char *name = strrchr (program_invocation_name, '/'); return name ? name + 1 : program_invocation_name; # else /* FIXME: What now? Miles suggests that it is better to use NULL, but currently the value is passed on directly to fputs_unlocked, so that requires more changes. */ # if __GNUC__ # warning No reasonable value to return # endif /* __GNUC__ */ return ""; # endif } #endif /* Output, if appropriate, a usage message for STATE to STREAM. FLAGS are from the set ARGP_HELP_*. */ void __argp_state_help (const struct argp_state *state, FILE *stream, unsigned flags) { if ((!state || ! (state->flags & ARGP_NO_ERRS)) && stream) { if (state && (state->flags & ARGP_LONG_ONLY)) flags |= ARGP_HELP_LONG_ONLY; _help (state ? state->root_argp : 0, state, stream, flags, state ? state->name : __argp_short_program_name ()); if (!state || ! (state->flags & ARGP_NO_EXIT)) { if (flags & ARGP_HELP_EXIT_ERR) exit (argp_err_exit_status); if (flags & ARGP_HELP_EXIT_OK) exit (0); } } } #ifdef weak_alias weak_alias (__argp_state_help, argp_state_help) #endif /* If appropriate, print the printf string FMT and following args, preceded by the program name and ':', to stderr, and followed by a "Try ... --help" message, then exit (1). */ void __argp_error (const struct argp_state *state, const char *fmt, ...) { if (!state || !(state->flags & ARGP_NO_ERRS)) { FILE *stream = state ? state->err_stream : stderr; if (stream) { va_list ap; #if _LIBC || (HAVE_FLOCKFILE && HAVE_FUNLOCKFILE) __flockfile (stream); #endif va_start (ap, fmt); #ifdef _LIBC char *buf; if (_IO_vasprintf (&buf, fmt, ap) < 0) buf = NULL; __fxprintf (stream, "%s: %s\n", state ? state->name : __argp_short_program_name (), buf); free (buf); #else fputs_unlocked (state ? state->name : __argp_short_program_name (), stream); putc_unlocked (':', stream); putc_unlocked (' ', stream); vfprintf (stream, fmt, ap); putc_unlocked ('\n', stream); #endif __argp_state_help (state, stream, ARGP_HELP_STD_ERR); va_end (ap); #if _LIBC || (HAVE_FLOCKFILE && HAVE_FUNLOCKFILE) __funlockfile (stream); #endif } } } #ifdef weak_alias weak_alias (__argp_error, argp_error) #endif /* Similar to the standard gnu error-reporting function error(), but will respect the ARGP_NO_EXIT and ARGP_NO_ERRS flags in STATE, and will print to STATE->err_stream. This is useful for argument parsing code that is shared between program startup (when exiting is desired) and runtime option parsing (when typically an error code is returned instead). The difference between this function and argp_error is that the latter is for *parsing errors*, and the former is for other problems that occur during parsing but don't reflect a (syntactic) problem with the input. */ void __argp_failure (const struct argp_state *state, int status, int errnum, const char *fmt, ...) { if (!state || !(state->flags & ARGP_NO_ERRS)) { FILE *stream = state ? state->err_stream : stderr; if (stream) { #if _LIBC || (HAVE_FLOCKFILE && HAVE_FUNLOCKFILE) __flockfile (stream); #endif #ifdef _LIBC __fxprintf (stream, "%s", state ? state->name : __argp_short_program_name ()); #else fputs_unlocked (state ? state->name : __argp_short_program_name (), stream); #endif if (fmt) { va_list ap; va_start (ap, fmt); #ifdef _LIBC char *buf; if (_IO_vasprintf (&buf, fmt, ap) < 0) buf = NULL; __fxprintf (stream, ": %s", buf); free (buf); #else putc_unlocked (':', stream); putc_unlocked (' ', stream); vfprintf (stream, fmt, ap); #endif va_end (ap); } if (errnum) { char buf[200]; #ifdef _LIBC __fxprintf (stream, ": %s", __strerror_r (errnum, buf, sizeof (buf))); #else char const *s = NULL; putc_unlocked (':', stream); putc_unlocked (' ', stream); # if HAVE_DECL_STRERROR_R # if STRERROR_R_CHAR_P s = __strerror_r (errnum, buf, sizeof buf); # else if (__strerror_r (errnum, buf, sizeof buf) == 0) s = buf; # endif # endif if (! s && ! (s = strerror (errnum))) s = dgettext (state->root_argp->argp_domain, "Unknown system error"); fputs_unlocked (s, stream); #endif } #if _LIBC if (_IO_fwide (stream, 0) > 0) putwc_unlocked (L'\n', stream); else #endif putc_unlocked ('\n', stream); #if _LIBC || (HAVE_FLOCKFILE && HAVE_FUNLOCKFILE) __funlockfile (stream); #endif if (status && (!state || !(state->flags & ARGP_NO_EXIT))) exit (status); } } } #ifdef weak_alias weak_alias (__argp_failure, argp_failure) #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/argp-fs-xinl.c0000644000175000017500000000317313004436754017056 00000000000000/* Real definitions for extern inline functions in argp-fmtstream.h Copyright (C) 1997-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifdef HAVE_CONFIG_H # include #endif #ifdef _LIBC # define ARGP_FS_EI #else # define ARGP_FS_EI _GL_EXTERN_INLINE #endif #undef __OPTIMIZE__ #define __OPTIMIZE__ 1 #include "argp-fmtstream.h" #if 0 /* Not exported. */ /* Add weak aliases. */ #if _LIBC - 0 && !defined (ARGP_FMTSTREAM_USE_LINEWRAP) && defined (weak_alias) weak_alias (__argp_fmtstream_putc, argp_fmtstream_putc) weak_alias (__argp_fmtstream_puts, argp_fmtstream_puts) weak_alias (__argp_fmtstream_write, argp_fmtstream_write) weak_alias (__argp_fmtstream_set_lmargin, argp_fmtstream_set_lmargin) weak_alias (__argp_fmtstream_set_rmargin, argp_fmtstream_set_rmargin) weak_alias (__argp_fmtstream_set_wmargin, argp_fmtstream_set_wmargin) weak_alias (__argp_fmtstream_point, argp_fmtstream_point) #endif #endif gnuastro-0.2.33-8a3b/bootstrapped/lib/argp-fmtstream.h0000644000175000017500000002660013004436754017505 00000000000000/* Word-wrapping and line-truncating streams. Copyright (C) 1997-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* This package emulates glibc 'line_wrap_stream' semantics for systems that don't have that. If the system does have it, it is just a wrapper for that. This header file is only used internally while compiling argp, and shouldn't be installed. */ #ifndef _ARGP_FMTSTREAM_H #define _ARGP_FMTSTREAM_H #include #include #include /* The __attribute__ feature is available in gcc versions 2.5 and later. The __-protected variants of the attributes 'format' and 'printf' are accepted by gcc versions 2.6.4 (effectively 2.7) and later. We enable _GL_ATTRIBUTE_FORMAT only if these are supported too, because gnulib and libintl do '#define printf __printf__' when they override the 'printf' function. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 7) # define _GL_ATTRIBUTE_FORMAT(spec) __attribute__ ((__format__ spec)) #else # define _GL_ATTRIBUTE_FORMAT(spec) /* empty */ #endif #if defined (__GNU_LIBRARY__) && defined (HAVE_LINEWRAP_H) /* line_wrap_stream is available, so use that. */ #define ARGP_FMTSTREAM_USE_LINEWRAP #endif #ifdef ARGP_FMTSTREAM_USE_LINEWRAP /* Just be a simple wrapper for line_wrap_stream; the semantics are *slightly* different, as line_wrap_stream doesn't actually make a new object, it just modifies the given stream (reversibly) to do line-wrapping. Since we control who uses this code, it doesn't matter. */ #include typedef FILE *argp_fmtstream_t; #define argp_make_fmtstream line_wrap_stream #define __argp_make_fmtstream line_wrap_stream #define argp_fmtstream_free line_unwrap_stream #define __argp_fmtstream_free line_unwrap_stream #define __argp_fmtstream_putc(fs,ch) putc(ch,fs) #define argp_fmtstream_putc(fs,ch) putc(ch,fs) #define __argp_fmtstream_puts(fs,str) fputs(str,fs) #define argp_fmtstream_puts(fs,str) fputs(str,fs) #define __argp_fmtstream_write(fs,str,len) fwrite(str,1,len,fs) #define argp_fmtstream_write(fs,str,len) fwrite(str,1,len,fs) #define __argp_fmtstream_printf fprintf #define argp_fmtstream_printf fprintf #define __argp_fmtstream_lmargin line_wrap_lmargin #define argp_fmtstream_lmargin line_wrap_lmargin #define __argp_fmtstream_set_lmargin line_wrap_set_lmargin #define argp_fmtstream_set_lmargin line_wrap_set_lmargin #define __argp_fmtstream_rmargin line_wrap_rmargin #define argp_fmtstream_rmargin line_wrap_rmargin #define __argp_fmtstream_set_rmargin line_wrap_set_rmargin #define argp_fmtstream_set_rmargin line_wrap_set_rmargin #define __argp_fmtstream_wmargin line_wrap_wmargin #define argp_fmtstream_wmargin line_wrap_wmargin #define __argp_fmtstream_set_wmargin line_wrap_set_wmargin #define argp_fmtstream_set_wmargin line_wrap_set_wmargin #define __argp_fmtstream_point line_wrap_point #define argp_fmtstream_point line_wrap_point #else /* !ARGP_FMTSTREAM_USE_LINEWRAP */ /* Guess we have to define our own version. */ struct argp_fmtstream { FILE *stream; /* The stream we're outputting to. */ size_t lmargin, rmargin; /* Left and right margins. */ ssize_t wmargin; /* Margin to wrap to, or -1 to truncate. */ /* Point in buffer to which we've processed for wrapping, but not output. */ size_t point_offs; /* Output column at POINT_OFFS, or -1 meaning 0 but don't add lmargin. */ ssize_t point_col; char *buf; /* Output buffer. */ char *p; /* Current end of text in BUF. */ char *end; /* Absolute end of BUF. */ }; typedef struct argp_fmtstream *argp_fmtstream_t; /* Return an argp_fmtstream that outputs to STREAM, and which prefixes lines written on it with LMARGIN spaces and limits them to RMARGIN columns total. If WMARGIN >= 0, words that extend past RMARGIN are wrapped by replacing the whitespace before them with a newline and WMARGIN spaces. Otherwise, chars beyond RMARGIN are simply dropped until a newline. Returns NULL if there was an error. */ extern argp_fmtstream_t __argp_make_fmtstream (FILE *__stream, size_t __lmargin, size_t __rmargin, ssize_t __wmargin); extern argp_fmtstream_t argp_make_fmtstream (FILE *__stream, size_t __lmargin, size_t __rmargin, ssize_t __wmargin); /* Flush __FS to its stream, and free it (but don't close the stream). */ extern void __argp_fmtstream_free (argp_fmtstream_t __fs); extern void argp_fmtstream_free (argp_fmtstream_t __fs); extern ssize_t __argp_fmtstream_printf (argp_fmtstream_t __fs, const char *__fmt, ...) _GL_ATTRIBUTE_FORMAT ((printf, 2, 3)); extern ssize_t argp_fmtstream_printf (argp_fmtstream_t __fs, const char *__fmt, ...) _GL_ATTRIBUTE_FORMAT ((printf, 2, 3)); #if _LIBC extern int __argp_fmtstream_putc (argp_fmtstream_t __fs, int __ch); extern int argp_fmtstream_putc (argp_fmtstream_t __fs, int __ch); extern int __argp_fmtstream_puts (argp_fmtstream_t __fs, const char *__str); extern int argp_fmtstream_puts (argp_fmtstream_t __fs, const char *__str); extern size_t __argp_fmtstream_write (argp_fmtstream_t __fs, const char *__str, size_t __len); extern size_t argp_fmtstream_write (argp_fmtstream_t __fs, const char *__str, size_t __len); #endif /* Access macros for various bits of state. */ #define argp_fmtstream_lmargin(__fs) ((__fs)->lmargin) #define argp_fmtstream_rmargin(__fs) ((__fs)->rmargin) #define argp_fmtstream_wmargin(__fs) ((__fs)->wmargin) #define __argp_fmtstream_lmargin argp_fmtstream_lmargin #define __argp_fmtstream_rmargin argp_fmtstream_rmargin #define __argp_fmtstream_wmargin argp_fmtstream_wmargin #if _LIBC /* Set __FS's left margin to LMARGIN and return the old value. */ extern size_t argp_fmtstream_set_lmargin (argp_fmtstream_t __fs, size_t __lmargin); extern size_t __argp_fmtstream_set_lmargin (argp_fmtstream_t __fs, size_t __lmargin); /* Set __FS's right margin to __RMARGIN and return the old value. */ extern size_t argp_fmtstream_set_rmargin (argp_fmtstream_t __fs, size_t __rmargin); extern size_t __argp_fmtstream_set_rmargin (argp_fmtstream_t __fs, size_t __rmargin); /* Set __FS's wrap margin to __WMARGIN and return the old value. */ extern size_t argp_fmtstream_set_wmargin (argp_fmtstream_t __fs, size_t __wmargin); extern size_t __argp_fmtstream_set_wmargin (argp_fmtstream_t __fs, size_t __wmargin); /* Return the column number of the current output point in __FS. */ extern size_t argp_fmtstream_point (argp_fmtstream_t __fs); extern size_t __argp_fmtstream_point (argp_fmtstream_t __fs); #endif /* Internal routines. */ extern void _argp_fmtstream_update (argp_fmtstream_t __fs); extern void __argp_fmtstream_update (argp_fmtstream_t __fs); extern int _argp_fmtstream_ensure (argp_fmtstream_t __fs, size_t __amount); extern int __argp_fmtstream_ensure (argp_fmtstream_t __fs, size_t __amount); #if !_LIBC || defined __OPTIMIZE__ /* Inline versions of above routines. */ #if !_LIBC #define __argp_fmtstream_putc argp_fmtstream_putc #define __argp_fmtstream_puts argp_fmtstream_puts #define __argp_fmtstream_write argp_fmtstream_write #define __argp_fmtstream_set_lmargin argp_fmtstream_set_lmargin #define __argp_fmtstream_set_rmargin argp_fmtstream_set_rmargin #define __argp_fmtstream_set_wmargin argp_fmtstream_set_wmargin #define __argp_fmtstream_point argp_fmtstream_point #define __argp_fmtstream_update _argp_fmtstream_update #define __argp_fmtstream_ensure _argp_fmtstream_ensure #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef ARGP_FS_EI # define ARGP_FS_EI _GL_INLINE #endif #endif #ifndef ARGP_FS_EI #define ARGP_FS_EI extern inline #endif ARGP_FS_EI size_t __argp_fmtstream_write (argp_fmtstream_t __fs, const char *__str, size_t __len) { if (__fs->p + __len <= __fs->end || __argp_fmtstream_ensure (__fs, __len)) { memcpy (__fs->p, __str, __len); __fs->p += __len; return __len; } else return 0; } ARGP_FS_EI int __argp_fmtstream_puts (argp_fmtstream_t __fs, const char *__str) { size_t __len = strlen (__str); if (__len) { size_t __wrote = __argp_fmtstream_write (__fs, __str, __len); return __wrote == __len ? 0 : -1; } else return 0; } ARGP_FS_EI int __argp_fmtstream_putc (argp_fmtstream_t __fs, int __ch) { if (__fs->p < __fs->end || __argp_fmtstream_ensure (__fs, 1)) return *__fs->p++ = __ch; else return EOF; } /* Set __FS's left margin to __LMARGIN and return the old value. */ ARGP_FS_EI size_t __argp_fmtstream_set_lmargin (argp_fmtstream_t __fs, size_t __lmargin) { size_t __old; if ((size_t) (__fs->p - __fs->buf) > __fs->point_offs) __argp_fmtstream_update (__fs); __old = __fs->lmargin; __fs->lmargin = __lmargin; return __old; } /* Set __FS's right margin to __RMARGIN and return the old value. */ ARGP_FS_EI size_t __argp_fmtstream_set_rmargin (argp_fmtstream_t __fs, size_t __rmargin) { size_t __old; if ((size_t) (__fs->p - __fs->buf) > __fs->point_offs) __argp_fmtstream_update (__fs); __old = __fs->rmargin; __fs->rmargin = __rmargin; return __old; } /* Set FS's wrap margin to __WMARGIN and return the old value. */ ARGP_FS_EI size_t __argp_fmtstream_set_wmargin (argp_fmtstream_t __fs, size_t __wmargin) { size_t __old; if ((size_t) (__fs->p - __fs->buf) > __fs->point_offs) __argp_fmtstream_update (__fs); __old = __fs->wmargin; __fs->wmargin = __wmargin; return __old; } /* Return the column number of the current output point in __FS. */ ARGP_FS_EI size_t __argp_fmtstream_point (argp_fmtstream_t __fs) { if ((size_t) (__fs->p - __fs->buf) > __fs->point_offs) __argp_fmtstream_update (__fs); return __fs->point_col >= 0 ? __fs->point_col : 0; } #if !_LIBC #undef __argp_fmtstream_putc #undef __argp_fmtstream_puts #undef __argp_fmtstream_write #undef __argp_fmtstream_set_lmargin #undef __argp_fmtstream_set_rmargin #undef __argp_fmtstream_set_wmargin #undef __argp_fmtstream_point #undef __argp_fmtstream_update #undef __argp_fmtstream_ensure _GL_INLINE_HEADER_END #endif #endif /* !_LIBC || __OPTIMIZE__ */ #endif /* ARGP_FMTSTREAM_USE_LINEWRAP */ #endif /* argp-fmtstream.h */ gnuastro-0.2.33-8a3b/bootstrapped/lib/argp-fmtstream.c0000644000175000017500000003166313004436754017505 00000000000000/* Word-wrapping and line-truncating streams Copyright (C) 1997-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* This package emulates glibc 'line_wrap_stream' semantics for systems that don't have that. */ #ifdef HAVE_CONFIG_H # include #endif #include #include #include #include #include #include "argp-fmtstream.h" #include "argp-namefrob.h" #ifndef ARGP_FMTSTREAM_USE_LINEWRAP #ifndef isblank #define isblank(ch) ((ch)==' ' || (ch)=='\t') #endif #ifdef _LIBC # include # include # define __vsnprintf(s, l, f, a) _IO_vsnprintf (s, l, f, a) #endif #define INIT_BUF_SIZE 200 #define PRINTF_SIZE_GUESS 150 /* Return an argp_fmtstream that outputs to STREAM, and which prefixes lines written on it with LMARGIN spaces and limits them to RMARGIN columns total. If WMARGIN >= 0, words that extend past RMARGIN are wrapped by replacing the whitespace before them with a newline and WMARGIN spaces. Otherwise, chars beyond RMARGIN are simply dropped until a newline. Returns NULL if there was an error. */ argp_fmtstream_t __argp_make_fmtstream (FILE *stream, size_t lmargin, size_t rmargin, ssize_t wmargin) { argp_fmtstream_t fs; fs = (struct argp_fmtstream *) malloc (sizeof (struct argp_fmtstream)); if (fs != NULL) { fs->stream = stream; fs->lmargin = lmargin; fs->rmargin = rmargin; fs->wmargin = wmargin; fs->point_col = 0; fs->point_offs = 0; fs->buf = (char *) malloc (INIT_BUF_SIZE); if (! fs->buf) { free (fs); fs = 0; } else { fs->p = fs->buf; fs->end = fs->buf + INIT_BUF_SIZE; } } return fs; } #if 0 /* Not exported. */ #ifdef weak_alias weak_alias (__argp_make_fmtstream, argp_make_fmtstream) #endif #endif /* Flush FS to its stream, and free it (but don't close the stream). */ void __argp_fmtstream_free (argp_fmtstream_t fs) { __argp_fmtstream_update (fs); if (fs->p > fs->buf) { #ifdef _LIBC __fxprintf (fs->stream, "%.*s", (int) (fs->p - fs->buf), fs->buf); #else fwrite_unlocked (fs->buf, 1, fs->p - fs->buf, fs->stream); #endif } free (fs->buf); free (fs); } #if 0 /* Not exported. */ #ifdef weak_alias weak_alias (__argp_fmtstream_free, argp_fmtstream_free) #endif #endif /* Process FS's buffer so that line wrapping is done from POINT_OFFS to the end of its buffer. This code is mostly from glibc stdio/linewrap.c. */ void __argp_fmtstream_update (argp_fmtstream_t fs) { char *buf, *nl; size_t len; /* Scan the buffer for newlines. */ buf = fs->buf + fs->point_offs; while (buf < fs->p) { size_t r; if (fs->point_col == 0 && fs->lmargin != 0) { /* We are starting a new line. Print spaces to the left margin. */ const size_t pad = fs->lmargin; if (fs->p + pad < fs->end) { /* We can fit in them in the buffer by moving the buffer text up and filling in the beginning. */ memmove (buf + pad, buf, fs->p - buf); fs->p += pad; /* Compensate for bigger buffer. */ memset (buf, ' ', pad); /* Fill in the spaces. */ buf += pad; /* Don't bother searching them. */ } else { /* No buffer space for spaces. Must flush. */ size_t i; for (i = 0; i < pad; i++) { #ifdef _LIBC if (_IO_fwide (fs->stream, 0) > 0) putwc_unlocked (L' ', fs->stream); else #endif putc_unlocked (' ', fs->stream); } } fs->point_col = pad; } len = fs->p - buf; nl = memchr (buf, '\n', len); if (fs->point_col < 0) fs->point_col = 0; if (!nl) { /* The buffer ends in a partial line. */ if (fs->point_col + len < fs->rmargin) { /* The remaining buffer text is a partial line and fits within the maximum line width. Advance point for the characters to be written and stop scanning. */ fs->point_col += len; break; } else /* Set the end-of-line pointer for the code below to the end of the buffer. */ nl = fs->p; } else if (fs->point_col + (nl - buf) < (ssize_t) fs->rmargin) { /* The buffer contains a full line that fits within the maximum line width. Reset point and scan the next line. */ fs->point_col = 0; buf = nl + 1; continue; } /* This line is too long. */ r = fs->rmargin - 1; if (fs->wmargin < 0) { /* Truncate the line by overwriting the excess with the newline and anything after it in the buffer. */ if (nl < fs->p) { memmove (buf + (r - fs->point_col), nl, fs->p - nl); fs->p -= buf + (r - fs->point_col) - nl; /* Reset point for the next line and start scanning it. */ fs->point_col = 0; buf += r + 1; /* Skip full line plus \n. */ } else { /* The buffer ends with a partial line that is beyond the maximum line width. Advance point for the characters written, and discard those past the max from the buffer. */ fs->point_col += len; fs->p -= fs->point_col - r; break; } } else { /* Do word wrap. Go to the column just past the maximum line width and scan back for the beginning of the word there. Then insert a line break. */ char *p, *nextline; int i; p = buf + (r + 1 - fs->point_col); while (p >= buf && !isblank ((unsigned char) *p)) --p; nextline = p + 1; /* This will begin the next line. */ if (nextline > buf) { /* Swallow separating blanks. */ if (p >= buf) do --p; while (p >= buf && isblank ((unsigned char) *p)); nl = p + 1; /* The newline will replace the first blank. */ } else { /* A single word that is greater than the maximum line width. Oh well. Put it on an overlong line by itself. */ p = buf + (r + 1 - fs->point_col); /* Find the end of the long word. */ if (p < nl) do ++p; while (p < nl && !isblank ((unsigned char) *p)); if (p == nl) { /* It already ends a line. No fussing required. */ fs->point_col = 0; buf = nl + 1; continue; } /* We will move the newline to replace the first blank. */ nl = p; /* Swallow separating blanks. */ do ++p; while (isblank ((unsigned char) *p)); /* The next line will start here. */ nextline = p; } /* Note: There are a bunch of tests below for NEXTLINE == BUF + LEN + 1; this case is where NL happens to fall at the end of the buffer, and NEXTLINE is in fact empty (and so we need not be careful to maintain its contents). */ if ((nextline == buf + len + 1 ? fs->end - nl < fs->wmargin + 1 : nextline - (nl + 1) < fs->wmargin) && fs->p > nextline) { /* The margin needs more blanks than we removed. */ if (fs->end - fs->p > fs->wmargin + 1) /* Make some space for them. */ { size_t mv = fs->p - nextline; memmove (nl + 1 + fs->wmargin, nextline, mv); nextline = nl + 1 + fs->wmargin; len = nextline + mv - buf; *nl++ = '\n'; } else /* Output the first line so we can use the space. */ { #ifdef _LIBC __fxprintf (fs->stream, "%.*s\n", (int) (nl - fs->buf), fs->buf); #else if (nl > fs->buf) fwrite_unlocked (fs->buf, 1, nl - fs->buf, fs->stream); putc_unlocked ('\n', fs->stream); #endif len += buf - fs->buf; nl = buf = fs->buf; } } else /* We can fit the newline and blanks in before the next word. */ *nl++ = '\n'; if (nextline - nl >= fs->wmargin || (nextline == buf + len + 1 && fs->end - nextline >= fs->wmargin)) /* Add blanks up to the wrap margin column. */ for (i = 0; i < fs->wmargin; ++i) *nl++ = ' '; else for (i = 0; i < fs->wmargin; ++i) #ifdef _LIBC if (_IO_fwide (fs->stream, 0) > 0) putwc_unlocked (L' ', fs->stream); else #endif putc_unlocked (' ', fs->stream); /* Copy the tail of the original buffer into the current buffer position. */ if (nl < nextline) memmove (nl, nextline, buf + len - nextline); len -= nextline - buf; /* Continue the scan on the remaining lines in the buffer. */ buf = nl; /* Restore bufp to include all the remaining text. */ fs->p = nl + len; /* Reset the counter of what has been output this line. If wmargin is 0, we want to avoid the lmargin getting added, so we set point_col to a magic value of -1 in that case. */ fs->point_col = fs->wmargin ? fs->wmargin : -1; } } /* Remember that we've scanned as far as the end of the buffer. */ fs->point_offs = fs->p - fs->buf; } /* Ensure that FS has space for AMOUNT more bytes in its buffer, either by growing the buffer, or by flushing it. True is returned iff we succeed. */ int __argp_fmtstream_ensure (struct argp_fmtstream *fs, size_t amount) { if ((size_t) (fs->end - fs->p) < amount) { ssize_t wrote; /* Flush FS's buffer. */ __argp_fmtstream_update (fs); #ifdef _LIBC __fxprintf (fs->stream, "%.*s", (int) (fs->p - fs->buf), fs->buf); wrote = fs->p - fs->buf; #else wrote = fwrite_unlocked (fs->buf, 1, fs->p - fs->buf, fs->stream); #endif if (wrote == fs->p - fs->buf) { fs->p = fs->buf; fs->point_offs = 0; } else { fs->p -= wrote; fs->point_offs -= wrote; memmove (fs->buf, fs->buf + wrote, fs->p - fs->buf); return 0; } if ((size_t) (fs->end - fs->buf) < amount) /* Gotta grow the buffer. */ { size_t old_size = fs->end - fs->buf; size_t new_size = old_size + amount; char *new_buf; if (new_size < old_size || ! (new_buf = realloc (fs->buf, new_size))) { __set_errno (ENOMEM); return 0; } fs->buf = new_buf; fs->end = new_buf + new_size; fs->p = fs->buf; } } return 1; } ssize_t __argp_fmtstream_printf (struct argp_fmtstream *fs, const char *fmt, ...) { int out; size_t avail; size_t size_guess = PRINTF_SIZE_GUESS; /* How much space to reserve. */ do { va_list args; if (! __argp_fmtstream_ensure (fs, size_guess)) return -1; va_start (args, fmt); avail = fs->end - fs->p; out = __vsnprintf (fs->p, avail, fmt, args); va_end (args); if ((size_t) out >= avail) size_guess = out + 1; } while ((size_t) out >= avail); fs->p += out; return out; } #if 0 /* Not exported. */ #ifdef weak_alias weak_alias (__argp_fmtstream_printf, argp_fmtstream_printf) #endif #endif #endif /* !ARGP_FMTSTREAM_USE_LINEWRAP */ gnuastro-0.2.33-8a3b/bootstrapped/lib/argp-eexst.c0000644000175000017500000000220613004436754016622 00000000000000/* Default definition for ARGP_ERR_EXIT_STATUS Copyright (C) 1997, 2009-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifdef HAVE_CONFIG_H # include #endif #include #include "argp.h" /* The exit status that argp will use when exiting due to a parsing error. If not defined or set by the user program, this defaults to EX_USAGE from . */ error_t argp_err_exit_status = EX_USAGE; gnuastro-0.2.33-8a3b/bootstrapped/lib/argp-ba.c0000644000175000017500000000310213004436754016050 00000000000000/* Default definition for ARGP_PROGRAM_BUG_ADDRESS. Copyright (C) 1996-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* If set by the user program, it should point to string that is the bug-reporting address for the program. It will be printed by argp_help if the ARGP_HELP_BUG_ADDR flag is set (as it is by various standard help messages), embedded in a sentence that says something like "Report bugs to ADDR." */ const char *argp_program_bug_address /* This variable should be zero-initialized. On most systems, putting it into BSS is sufficient. Not so on Mac OS X 10.3 and 10.4, see . */ #if defined __ELF__ /* On ELF systems, variables in BSS behave well. */ #else = (const char *) 0 #endif ; gnuastro-0.2.33-8a3b/bootstrapped/lib/argp.h0000644000175000017500000006751613004436754015520 00000000000000/* Hierarchical argument parsing, layered over getopt. Copyright (C) 1995-2016 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _ARGP_H #define _ARGP_H #include #include #include #include #define __need_error_t #include #ifndef __THROW # define __THROW #endif #ifndef __NTH # define __NTH(fct) fct __THROW #endif /* The __attribute__ feature is available in gcc versions 2.5 and later. The __-protected variants of the attributes 'format' and 'printf' are accepted by gcc versions 2.6.4 (effectively 2.7) and later. We enable _GL_ATTRIBUTE_FORMAT only if these are supported too, because gnulib and libintl do '#define printf __printf__' when they override the 'printf' function. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 7) # define _GL_ATTRIBUTE_FORMAT(spec) __attribute__ ((__format__ spec)) #else # define _GL_ATTRIBUTE_FORMAT(spec) /* empty */ #endif /* GCC 2.95 and later have "__restrict"; C99 compilers have "restrict", and "configure" may have defined "restrict". Other compilers use __restrict, __restrict__, and _Restrict, and 'configure' might #define 'restrict' to those words. */ #ifndef __restrict # if ! (2 < __GNUC__ || (2 == __GNUC__ && 95 <= __GNUC_MINOR__)) # if 199901L <= __STDC_VERSION__ # define __restrict restrict # else # define __restrict # endif # endif #endif #ifndef __error_t_defined typedef int error_t; # define __error_t_defined #endif #ifdef __cplusplus extern "C" { #endif /* A description of a particular option. A pointer to an array of these is passed in the OPTIONS field of an argp structure. Each option entry can correspond to one long option and/or one short option; more names for the same option can be added by following an entry in an option array with options having the OPTION_ALIAS flag set. */ struct argp_option { /* The long option name. For more than one name for the same option, you can use following options with the OPTION_ALIAS flag set. */ const char *name; /* What key is returned for this option. If > 0 and printable, then it's also accepted as a short option. */ int key; /* If non-NULL, this is the name of the argument associated with this option, which is required unless the OPTION_ARG_OPTIONAL flag is set. */ const char *arg; /* OPTION_ flags. */ int flags; /* The doc string for this option. If both NAME and KEY are 0, This string will be printed outdented from the normal option column, making it useful as a group header (it will be the first thing printed in its group); in this usage, it's conventional to end the string with a ':'. Write the initial value as N_("TEXT") if you want xgettext to collect it into a POT file. */ const char *doc; /* The group this option is in. In a long help message, options are sorted alphabetically within each group, and the groups presented in the order 0, 1, 2, ..., n, -m, ..., -2, -1. Every entry in an options array with if this field 0 will inherit the group number of the previous entry, or zero if it's the first one, unless its a group header (NAME and KEY both 0), in which case, the previous entry + 1 is the default. Automagic options such as --help are put into group -1. */ int group; }; /* The argument associated with this option is optional. */ #define OPTION_ARG_OPTIONAL 0x1 /* This option isn't displayed in any help messages. */ #define OPTION_HIDDEN 0x2 /* This option is an alias for the closest previous non-alias option. This means that it will be displayed in the same help entry, and will inherit fields other than NAME and KEY from the aliased option. */ #define OPTION_ALIAS 0x4 /* This option isn't actually an option (and so should be ignored by the actual option parser), but rather an arbitrary piece of documentation that should be displayed in much the same manner as the options. If this flag is set, then the option NAME field is displayed unmodified (e.g., no '--' prefix is added) at the left-margin (where a *short* option would normally be displayed), and the documentation string in the normal place. The NAME field will be translated using gettext, unless OPTION_NO_TRANS is set (see below). For purposes of sorting, any leading whitespace and punctuation is ignored, except that if the first non-whitespace character is not '-', this entry is displayed after all options (and OPTION_DOC entries with a leading '-') in the same group. */ #define OPTION_DOC 0x8 /* This option shouldn't be included in "long" usage messages (but is still included in help messages). This is mainly intended for options that are completely documented in an argp's ARGS_DOC field, in which case including the option in the generic usage list would be redundant. For instance, if ARGS_DOC is "FOO BAR\n-x BLAH", and the '-x' option's purpose is to distinguish these two cases, -x should probably be marked OPTION_NO_USAGE. */ #define OPTION_NO_USAGE 0x10 /* Valid only in conjunction with OPTION_DOC. This option disables translation of option name. */ #define OPTION_NO_TRANS 0x20 struct argp; /* fwd declare this type */ struct argp_state; /* " */ struct argp_child; /* " */ /* The type of a pointer to an argp parsing function. */ typedef error_t (*argp_parser_t) (int __key, char *__arg, struct argp_state *__state); /* What to return for unrecognized keys. For special ARGP_KEY_ keys, such returns will simply be ignored. For user keys, this error will be turned into EINVAL (if the call to argp_parse is such that errors are propagated back to the user instead of exiting); returning EINVAL itself would result in an immediate stop to parsing in *all* cases. */ #define ARGP_ERR_UNKNOWN E2BIG /* Hurd should never need E2BIG. XXX */ /* Special values for the KEY argument to an argument parsing function. ARGP_ERR_UNKNOWN should be returned if they aren't understood. The sequence of keys to a parsing function is either (where each uppercased word should be prefixed by 'ARGP_KEY_' and opt is a user key): INIT opt... NO_ARGS END SUCCESS -- No non-option arguments at all or INIT (opt | ARG)... END SUCCESS -- All non-option args parsed or INIT (opt | ARG)... SUCCESS -- Some non-option arg unrecognized The third case is where every parser returned ARGP_KEY_UNKNOWN for an argument, in which case parsing stops at that argument (returning the unparsed arguments to the caller of argp_parse if requested, or stopping with an error message if not). If an error occurs (either detected by argp, or because the parsing function returned an error value), then the parser is called with ARGP_KEY_ERROR, and no further calls are made. */ /* This is not an option at all, but rather a command line argument. If a parser receiving this key returns success, the fact is recorded, and the ARGP_KEY_NO_ARGS case won't be used. HOWEVER, if while processing the argument, a parser function decrements the NEXT field of the state it's passed, the option won't be considered processed; this is to allow you to actually modify the argument (perhaps into an option), and have it processed again. */ #define ARGP_KEY_ARG 0 /* There are remaining arguments not parsed by any parser, which may be found starting at (STATE->argv + STATE->next). If success is returned, but STATE->next left untouched, it's assumed that all arguments were consume, otherwise, the parser should adjust STATE->next to reflect any arguments consumed. */ #define ARGP_KEY_ARGS 0x1000006 /* There are no more command line arguments at all. */ #define ARGP_KEY_END 0x1000001 /* Because it's common to want to do some special processing if there aren't any non-option args, user parsers are called with this key if they didn't successfully process any non-option arguments. Called just before ARGP_KEY_END (where more general validity checks on previously parsed arguments can take place). */ #define ARGP_KEY_NO_ARGS 0x1000002 /* Passed in before any parsing is done. Afterwards, the values of each element of the CHILD_INPUT field, if any, in the state structure is copied to each child's state to be the initial value of the INPUT field. */ #define ARGP_KEY_INIT 0x1000003 /* Use after all other keys, including SUCCESS & END. */ #define ARGP_KEY_FINI 0x1000007 /* Passed in when parsing has successfully been completed (even if there are still arguments remaining). */ #define ARGP_KEY_SUCCESS 0x1000004 /* Passed in if an error occurs. */ #define ARGP_KEY_ERROR 0x1000005 /* An argp structure contains a set of options declarations, a function to deal with parsing one, documentation string, a possible vector of child argp's, and perhaps a function to filter help output. When actually parsing options, getopt is called with the union of all the argp structures chained together through their CHILD pointers, with conflicts being resolved in favor of the first occurrence in the chain. */ struct argp { /* An array of argp_option structures, terminated by an entry with both NAME and KEY having a value of 0. */ const struct argp_option *options; /* What to do with an option from this structure. KEY is the key associated with the option, and ARG is any associated argument (NULL if none was supplied). If KEY isn't understood, ARGP_ERR_UNKNOWN should be returned. If a non-zero, non-ARGP_ERR_UNKNOWN value is returned, then parsing is stopped immediately, and that value is returned from argp_parse(). For special (non-user-supplied) values of KEY, see the ARGP_KEY_ definitions below. */ argp_parser_t parser; /* A string describing what other arguments are wanted by this program. It is only used by argp_usage to print the "Usage:" message. If it contains newlines, the strings separated by them are considered alternative usage patterns, and printed on separate lines (lines after the first are prefix by " or: " instead of "Usage:"). */ const char *args_doc; /* If non-NULL, a string containing extra text to be printed before and after the options in a long help message (separated by a vertical tab '\v' character). Write the initial value as N_("BEFORE-TEXT") "\v" N_("AFTER-TEXT") if you want xgettext to collect the two pieces of text into a POT file. */ const char *doc; /* A vector of argp_children structures, terminated by a member with a 0 argp field, pointing to child argps should be parsed with this one. Any conflicts are resolved in favor of this argp, or early argps in the CHILDREN list. This field is useful if you use libraries that supply their own argp structure, which you want to use in conjunction with your own. */ const struct argp_child *children; /* If non-zero, this should be a function to filter the output of help messages. KEY is either a key from an option, in which case TEXT is that option's help text, or a special key from the ARGP_KEY_HELP_ defines, below, describing which other help text TEXT is. The function should return either TEXT, if it should be used as-is, a replacement string, which should be malloced, and will be freed by argp, or NULL, meaning "print nothing". The value for TEXT is *after* any translation has been done, so if any of the replacement text also needs translation, that should be done by the filter function. INPUT is either the input supplied to argp_parse, or NULL, if argp_help was called directly. */ char *(*help_filter) (int __key, const char *__text, void *__input); /* If non-zero the strings used in the argp library are translated using the domain described by this string. Otherwise the currently installed default domain is used. */ const char *argp_domain; }; /* Possible KEY arguments to a help filter function. */ #define ARGP_KEY_HELP_PRE_DOC 0x2000001 /* Help text preceding options. */ #define ARGP_KEY_HELP_POST_DOC 0x2000002 /* Help text following options. */ #define ARGP_KEY_HELP_HEADER 0x2000003 /* Option header string. */ #define ARGP_KEY_HELP_EXTRA 0x2000004 /* After all other documentation; TEXT is NULL for this key. */ /* Explanatory note emitted when duplicate option arguments have been suppressed. */ #define ARGP_KEY_HELP_DUP_ARGS_NOTE 0x2000005 #define ARGP_KEY_HELP_ARGS_DOC 0x2000006 /* Argument doc string. */ /* When an argp has a non-zero CHILDREN field, it should point to a vector of argp_child structures, each of which describes a subsidiary argp. */ struct argp_child { /* The child parser. */ const struct argp *argp; /* Flags for this child. */ int flags; /* If non-zero, an optional header to be printed in help output before the child options. As a side-effect, a non-zero value forces the child options to be grouped together; to achieve this effect without actually printing a header string, use a value of "". */ const char *header; /* Where to group the child options relative to the other ("consolidated") options in the parent argp; the values are the same as the GROUP field in argp_option structs, but all child-groupings follow parent options at a particular group level. If both this field and HEADER are zero, then they aren't grouped at all, but rather merged with the parent options (merging the child's grouping levels with the parents). */ int group; }; /* Parsing state. This is provided to parsing functions called by argp, which may examine and, as noted, modify fields. */ struct argp_state { /* The top level ARGP being parsed. */ const struct argp *root_argp; /* The argument vector being parsed. May be modified. */ int argc; char **argv; /* The index in ARGV of the next arg that to be parsed. May be modified. */ int next; /* The flags supplied to argp_parse. May be modified. */ unsigned flags; /* While calling a parsing function with a key of ARGP_KEY_ARG, this is the number of the current arg, starting at zero, and incremented after each such call returns. At all other times, this is the number of such arguments that have been processed. */ unsigned arg_num; /* If non-zero, the index in ARGV of the first argument following a special '--' argument (which prevents anything following being interpreted as an option). Only set once argument parsing has proceeded past this point. */ int quoted; /* An arbitrary pointer passed in from the user. */ void *input; /* Values to pass to child parsers. This vector will be the same length as the number of children for the current parser. */ void **child_inputs; /* For the parser's use. Initialized to 0. */ void *hook; /* The name used when printing messages. This is initialized to ARGV[0], or PROGRAM_INVOCATION_NAME if that is unavailable. */ char *name; /* Streams used when argp prints something. */ FILE *err_stream; /* For errors; initialized to stderr. */ FILE *out_stream; /* For information; initialized to stdout. */ void *pstate; /* Private, for use by argp. */ }; /* Flags for argp_parse (note that the defaults are those that are convenient for program command line parsing): */ /* Don't ignore the first element of ARGV. Normally (and always unless ARGP_NO_ERRS is set) the first element of the argument vector is skipped for option parsing purposes, as it corresponds to the program name in a command line. */ #define ARGP_PARSE_ARGV0 0x01 /* Don't print error messages for unknown options to stderr; unless this flag is set, ARGP_PARSE_ARGV0 is ignored, as ARGV[0] is used as the program name in the error messages. This flag implies ARGP_NO_EXIT (on the assumption that silent exiting upon errors is bad behaviour). */ #define ARGP_NO_ERRS 0x02 /* Don't parse any non-option args. Normally non-option args are parsed by calling the parse functions with a key of ARGP_KEY_ARG, and the actual arg as the value. Since it's impossible to know which parse function wants to handle it, each one is called in turn, until one returns 0 or an error other than ARGP_ERR_UNKNOWN; if an argument is handled by no one, the argp_parse returns prematurely (but with a return value of 0). If all args have been parsed without error, all parsing functions are called one last time with a key of ARGP_KEY_END. This flag needn't normally be set, as the normal behavior is to stop parsing as soon as some argument can't be handled. */ #define ARGP_NO_ARGS 0x04 /* Parse options and arguments in the same order they occur on the command line -- normally they're rearranged so that all options come first. */ #define ARGP_IN_ORDER 0x08 /* Don't provide the standard long option --help, which causes usage and option help information to be output to stdout, and exit (0) called. */ #define ARGP_NO_HELP 0x10 /* Don't exit on errors (they may still result in error messages). */ #define ARGP_NO_EXIT 0x20 /* Use the gnu getopt "long-only" rules for parsing arguments. */ #define ARGP_LONG_ONLY 0x40 /* Turns off any message-printing/exiting options. */ #define ARGP_SILENT (ARGP_NO_EXIT | ARGP_NO_ERRS | ARGP_NO_HELP) /* Parse the options strings in ARGC & ARGV according to the options in ARGP. FLAGS is one of the ARGP_ flags above. If ARG_INDEX is non-NULL, the index in ARGV of the first unparsed option is returned in it. If an unknown option is present, ARGP_ERR_UNKNOWN is returned; if some parser routine returned a non-zero value, it is returned; otherwise 0 is returned. This function may also call exit unless the ARGP_NO_HELP flag is set. INPUT is a pointer to a value to be passed in to the parser. */ extern error_t argp_parse (const struct argp *__restrict __argp, int /*argc*/, char **__restrict /*argv*/, unsigned __flags, int *__restrict __arg_index, void *__restrict __input); extern error_t __argp_parse (const struct argp *__restrict __argp, int /*argc*/, char **__restrict /*argv*/, unsigned __flags, int *__restrict __arg_index, void *__restrict __input); /* Global variables. */ /* GNULIB makes sure both program_invocation_name and program_invocation_short_name are available */ #ifdef GNULIB_PROGRAM_INVOCATION_NAME extern char *program_invocation_name; # undef HAVE_DECL_PROGRAM_INVOCATION_NAME # define HAVE_DECL_PROGRAM_INVOCATION_NAME 1 #endif #ifdef GNULIB_PROGRAM_INVOCATION_SHORT_NAME extern char *program_invocation_short_name; # undef HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME # define HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME 1 #endif /* If defined or set by the user program to a non-zero value, then a default option --version is added (unless the ARGP_NO_HELP flag is used), which will print this string followed by a newline and exit (unless the ARGP_NO_EXIT flag is used). Overridden by ARGP_PROGRAM_VERSION_HOOK. */ extern const char *argp_program_version; /* If defined or set by the user program to a non-zero value, then a default option --version is added (unless the ARGP_NO_HELP flag is used), which calls this function with a stream to print the version to and a pointer to the current parsing state, and then exits (unless the ARGP_NO_EXIT flag is used). This variable takes precedent over ARGP_PROGRAM_VERSION. */ extern void (*argp_program_version_hook) (FILE *__restrict __stream, struct argp_state *__restrict __state); /* If defined or set by the user program, it should point to string that is the bug-reporting address for the program. It will be printed by argp_help if the ARGP_HELP_BUG_ADDR flag is set (as it is by various standard help messages), embedded in a sentence that says something like "Report bugs to ADDR." */ extern const char *argp_program_bug_address; /* The exit status that argp will use when exiting due to a parsing error. If not defined or set by the user program, this defaults to EX_USAGE from . */ extern error_t argp_err_exit_status; /* Flags for argp_help. */ #define ARGP_HELP_USAGE 0x01 /* a Usage: message. */ #define ARGP_HELP_SHORT_USAGE 0x02 /* " but don't actually print options. */ #define ARGP_HELP_SEE 0x04 /* a "Try ... for more help" message. */ #define ARGP_HELP_LONG 0x08 /* a long help message. */ #define ARGP_HELP_PRE_DOC 0x10 /* doc string preceding long help. */ #define ARGP_HELP_POST_DOC 0x20 /* doc string following long help. */ #define ARGP_HELP_DOC (ARGP_HELP_PRE_DOC | ARGP_HELP_POST_DOC) #define ARGP_HELP_BUG_ADDR 0x40 /* bug report address */ #define ARGP_HELP_LONG_ONLY 0x80 /* modify output appropriately to reflect ARGP_LONG_ONLY mode. */ /* These ARGP_HELP flags are only understood by argp_state_help. */ #define ARGP_HELP_EXIT_ERR 0x100 /* Call exit(1) instead of returning. */ #define ARGP_HELP_EXIT_OK 0x200 /* Call exit(0) instead of returning. */ /* The standard thing to do after a program command line parsing error, if an error message has already been printed. */ #define ARGP_HELP_STD_ERR \ (ARGP_HELP_SEE | ARGP_HELP_EXIT_ERR) /* The standard thing to do after a program command line parsing error, if no more specific error message has been printed. */ #define ARGP_HELP_STD_USAGE \ (ARGP_HELP_SHORT_USAGE | ARGP_HELP_SEE | ARGP_HELP_EXIT_ERR) /* The standard thing to do in response to a --help option. */ #define ARGP_HELP_STD_HELP \ (ARGP_HELP_SHORT_USAGE | ARGP_HELP_LONG | ARGP_HELP_EXIT_OK \ | ARGP_HELP_DOC | ARGP_HELP_BUG_ADDR) /* Output a usage message for ARGP to STREAM. FLAGS are from the set ARGP_HELP_*. */ extern void argp_help (const struct argp *__restrict __argp, FILE *__restrict __stream, unsigned __flags, char *__restrict __name); extern void __argp_help (const struct argp *__restrict __argp, FILE *__restrict __stream, unsigned __flags, char *__name); /* The following routines are intended to be called from within an argp parsing routine (thus taking an argp_state structure as the first argument). They may or may not print an error message and exit, depending on the flags in STATE -- in any case, the caller should be prepared for them *not* to exit, and should return an appropriate error after calling them. [argp_usage & argp_error should probably be called argp_state_..., but they're used often enough that they should be short] */ /* Output, if appropriate, a usage message for STATE to STREAM. FLAGS are from the set ARGP_HELP_*. */ extern void argp_state_help (const struct argp_state *__restrict __state, FILE *__restrict __stream, unsigned int __flags); extern void __argp_state_help (const struct argp_state *__restrict __state, FILE *__restrict __stream, unsigned int __flags); #if _LIBC /* Possibly output the standard usage message for ARGP to stderr and exit. */ extern void argp_usage (const struct argp_state *__state); extern void __argp_usage (const struct argp_state *__state); #endif /* If appropriate, print the printf string FMT and following args, preceded by the program name and ':', to stderr, and followed by a "Try ... --help" message, then exit (1). */ extern void argp_error (const struct argp_state *__restrict __state, const char *__restrict __fmt, ...) _GL_ATTRIBUTE_FORMAT ((__printf__, 2, 3)); extern void __argp_error (const struct argp_state *__restrict __state, const char *__restrict __fmt, ...) _GL_ATTRIBUTE_FORMAT ((__printf__, 2, 3)); /* Similar to the standard gnu error-reporting function error(), but will respect the ARGP_NO_EXIT and ARGP_NO_ERRS flags in STATE, and will print to STATE->err_stream. This is useful for argument parsing code that is shared between program startup (when exiting is desired) and runtime option parsing (when typically an error code is returned instead). The difference between this function and argp_error is that the latter is for *parsing errors*, and the former is for other problems that occur during parsing but don't reflect a (syntactic) problem with the input. */ extern void argp_failure (const struct argp_state *__restrict __state, int __status, int __errnum, const char *__restrict __fmt, ...) _GL_ATTRIBUTE_FORMAT ((__printf__, 4, 5)); extern void __argp_failure (const struct argp_state *__restrict __state, int __status, int __errnum, const char *__restrict __fmt, ...) _GL_ATTRIBUTE_FORMAT ((__printf__, 4, 5)); #if _LIBC /* Returns true if the option OPT is a valid short option. */ extern int _option_is_short (const struct argp_option *__opt) __THROW; extern int __option_is_short (const struct argp_option *__opt) __THROW; /* Returns true if the option OPT is in fact the last (unused) entry in an options array. */ extern int _option_is_end (const struct argp_option *__opt) __THROW; extern int __option_is_end (const struct argp_option *__opt) __THROW; #endif /* Return the input field for ARGP in the parser corresponding to STATE; used by the help routines. */ extern void *_argp_input (const struct argp *__restrict __argp, const struct argp_state *__restrict __state) __THROW; extern void *__argp_input (const struct argp *__restrict __argp, const struct argp_state *__restrict __state) __THROW; #if !_LIBC || defined __USE_EXTERN_INLINES # if !_LIBC # define __argp_usage argp_usage # define __argp_state_help argp_state_help # define __option_is_short _option_is_short # define __option_is_end _option_is_end #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN # ifndef ARGP_EI # define ARGP_EI _GL_INLINE # endif # endif # ifndef ARGP_EI # define ARGP_EI __extern_inline # endif ARGP_EI void __argp_usage (const struct argp_state *__state) { __argp_state_help (__state, stderr, ARGP_HELP_STD_USAGE); } ARGP_EI int __NTH (__option_is_short (const struct argp_option *__opt)) { if (__opt->flags & OPTION_DOC) return 0; else { int __key = __opt->key; return __key > 0 && __key <= UCHAR_MAX && isprint (__key); } } ARGP_EI int __NTH (__option_is_end (const struct argp_option *__opt)) { return !__opt->key && !__opt->name && !__opt->doc && !__opt->group; } # if !_LIBC # undef __argp_usage # undef __argp_state_help # undef __option_is_short # undef __option_is_end _GL_INLINE_HEADER_END # endif #endif /* Use extern inlines. */ #ifdef __cplusplus } #endif #endif /* argp.h */ gnuastro-0.2.33-8a3b/bootstrapped/lib/alloca.c0000644000175000017500000003445413004436754016010 00000000000000/* alloca.c -- allocate automatically reclaimed memory (Mostly) portable public-domain implementation -- D A Gwyn This implementation of the PWB library alloca function, which is used to allocate space off the run-time stack so that it is automatically reclaimed upon procedure exit, was inspired by discussions with J. Q. Johnson of Cornell. J.Otto Tennant contributed the Cray support. There are some preprocessor constants that can be defined when compiling for your specific system, for improved efficiency; however, the defaults should be okay. The general concept of this implementation is to keep track of all alloca-allocated blocks, and reclaim any that are found to be deeper in the stack than the current invocation. This heuristic does not reclaim storage as soon as it becomes invalid, but it will do so eventually. As a special case, alloca(0) reclaims storage without allocating any. It is a good idea to use alloca(0) in your main control loop, etc. to force garbage collection. */ #include #include #include #include #ifdef emacs # include "lisp.h" # include "blockinput.h" # ifdef EMACS_FREE # undef free # define free EMACS_FREE # endif #else # define memory_full() abort () #endif /* If compiling with GCC 2, this file's not needed. */ #if !defined (__GNUC__) || __GNUC__ < 2 /* If someone has defined alloca as a macro, there must be some other way alloca is supposed to work. */ # ifndef alloca # ifdef emacs # ifdef static /* actually, only want this if static is defined as "" -- this is for usg, in which emacs must undefine static in order to make unexec workable */ # ifndef STACK_DIRECTION you lose -- must know STACK_DIRECTION at compile-time /* Using #error here is not wise since this file should work for old and obscure compilers. */ # endif /* STACK_DIRECTION undefined */ # endif /* static */ # endif /* emacs */ /* If your stack is a linked list of frames, you have to provide an "address metric" ADDRESS_FUNCTION macro. */ # if defined (CRAY) && defined (CRAY_STACKSEG_END) long i00afunc (); # define ADDRESS_FUNCTION(arg) (char *) i00afunc (&(arg)) # else # define ADDRESS_FUNCTION(arg) &(arg) # endif /* Define STACK_DIRECTION if you know the direction of stack growth for your system; otherwise it will be automatically deduced at run-time. STACK_DIRECTION > 0 => grows toward higher addresses STACK_DIRECTION < 0 => grows toward lower addresses STACK_DIRECTION = 0 => direction of growth unknown */ # ifndef STACK_DIRECTION # define STACK_DIRECTION 0 /* Direction unknown. */ # endif # if STACK_DIRECTION != 0 # define STACK_DIR STACK_DIRECTION /* Known at compile-time. */ # else /* STACK_DIRECTION == 0; need run-time code. */ static int stack_dir; /* 1 or -1 once known. */ # define STACK_DIR stack_dir static int find_stack_direction (int *addr, int depth) { int dir, dummy = 0; if (! addr) addr = &dummy; *addr = addr < &dummy ? 1 : addr == &dummy ? 0 : -1; dir = depth ? find_stack_direction (addr, depth - 1) : 0; return dir + dummy; } # endif /* STACK_DIRECTION == 0 */ /* An "alloca header" is used to: (a) chain together all alloca'ed blocks; (b) keep track of stack depth. It is very important that sizeof(header) agree with malloc alignment chunk size. The following default should work okay. */ # ifndef ALIGN_SIZE # define ALIGN_SIZE sizeof(double) # endif typedef union hdr { char align[ALIGN_SIZE]; /* To force sizeof(header). */ struct { union hdr *next; /* For chaining headers. */ char *deep; /* For stack depth measure. */ } h; } header; static header *last_alloca_header = NULL; /* -> last alloca header. */ /* Return a pointer to at least SIZE bytes of storage, which will be automatically reclaimed upon exit from the procedure that called alloca. Originally, this space was supposed to be taken from the current stack frame of the caller, but that method cannot be made to work for some implementations of C, for example under Gould's UTX/32. */ void * alloca (size_t size) { auto char probe; /* Probes stack depth: */ register char *depth = ADDRESS_FUNCTION (probe); # if STACK_DIRECTION == 0 if (STACK_DIR == 0) /* Unknown growth direction. */ STACK_DIR = find_stack_direction (NULL, (size & 1) + 20); # endif /* Reclaim garbage, defined as all alloca'd storage that was allocated from deeper in the stack than currently. */ { register header *hp; /* Traverses linked list. */ # ifdef emacs BLOCK_INPUT; # endif for (hp = last_alloca_header; hp != NULL;) if ((STACK_DIR > 0 && hp->h.deep > depth) || (STACK_DIR < 0 && hp->h.deep < depth)) { register header *np = hp->h.next; free (hp); /* Collect garbage. */ hp = np; /* -> next header. */ } else break; /* Rest are not deeper. */ last_alloca_header = hp; /* -> last valid storage. */ # ifdef emacs UNBLOCK_INPUT; # endif } if (size == 0) return NULL; /* No allocation required. */ /* Allocate combined header + user data storage. */ { /* Address of header. */ register header *new; size_t combined_size = sizeof (header) + size; if (combined_size < sizeof (header)) memory_full (); new = malloc (combined_size); if (! new) memory_full (); new->h.next = last_alloca_header; new->h.deep = depth; last_alloca_header = new; /* User storage begins just after header. */ return (void *) (new + 1); } } # if defined (CRAY) && defined (CRAY_STACKSEG_END) # ifdef DEBUG_I00AFUNC # include # endif # ifndef CRAY_STACK # define CRAY_STACK # ifndef CRAY2 /* Stack structures for CRAY-1, CRAY X-MP, and CRAY Y-MP */ struct stack_control_header { long shgrow:32; /* Number of times stack has grown. */ long shaseg:32; /* Size of increments to stack. */ long shhwm:32; /* High water mark of stack. */ long shsize:32; /* Current size of stack (all segments). */ }; /* The stack segment linkage control information occurs at the high-address end of a stack segment. (The stack grows from low addresses to high addresses.) The initial part of the stack segment linkage control information is 0200 (octal) words. This provides for register storage for the routine which overflows the stack. */ struct stack_segment_linkage { long ss[0200]; /* 0200 overflow words. */ long sssize:32; /* Number of words in this segment. */ long ssbase:32; /* Offset to stack base. */ long:32; long sspseg:32; /* Offset to linkage control of previous segment of stack. */ long:32; long sstcpt:32; /* Pointer to task common address block. */ long sscsnm; /* Private control structure number for microtasking. */ long ssusr1; /* Reserved for user. */ long ssusr2; /* Reserved for user. */ long sstpid; /* Process ID for pid based multi-tasking. */ long ssgvup; /* Pointer to multitasking thread giveup. */ long sscray[7]; /* Reserved for Cray Research. */ long ssa0; long ssa1; long ssa2; long ssa3; long ssa4; long ssa5; long ssa6; long ssa7; long sss0; long sss1; long sss2; long sss3; long sss4; long sss5; long sss6; long sss7; }; # else /* CRAY2 */ /* The following structure defines the vector of words returned by the STKSTAT library routine. */ struct stk_stat { long now; /* Current total stack size. */ long maxc; /* Amount of contiguous space which would be required to satisfy the maximum stack demand to date. */ long high_water; /* Stack high-water mark. */ long overflows; /* Number of stack overflow ($STKOFEN) calls. */ long hits; /* Number of internal buffer hits. */ long extends; /* Number of block extensions. */ long stko_mallocs; /* Block allocations by $STKOFEN. */ long underflows; /* Number of stack underflow calls ($STKRETN). */ long stko_free; /* Number of deallocations by $STKRETN. */ long stkm_free; /* Number of deallocations by $STKMRET. */ long segments; /* Current number of stack segments. */ long maxs; /* Maximum number of stack segments so far. */ long pad_size; /* Stack pad size. */ long current_address; /* Current stack segment address. */ long current_size; /* Current stack segment size. This number is actually corrupted by STKSTAT to include the fifteen word trailer area. */ long initial_address; /* Address of initial segment. */ long initial_size; /* Size of initial segment. */ }; /* The following structure describes the data structure which trails any stack segment. I think that the description in 'asdef' is out of date. I only describe the parts that I am sure about. */ struct stk_trailer { long this_address; /* Address of this block. */ long this_size; /* Size of this block (does not include this trailer). */ long unknown2; long unknown3; long link; /* Address of trailer block of previous segment. */ long unknown5; long unknown6; long unknown7; long unknown8; long unknown9; long unknown10; long unknown11; long unknown12; long unknown13; long unknown14; }; # endif /* CRAY2 */ # endif /* not CRAY_STACK */ # ifdef CRAY2 /* Determine a "stack measure" for an arbitrary ADDRESS. I doubt that "lint" will like this much. */ static long i00afunc (long *address) { struct stk_stat status; struct stk_trailer *trailer; long *block, size; long result = 0; /* We want to iterate through all of the segments. The first step is to get the stack status structure. We could do this more quickly and more directly, perhaps, by referencing the $LM00 common block, but I know that this works. */ STKSTAT (&status); /* Set up the iteration. */ trailer = (struct stk_trailer *) (status.current_address + status.current_size - 15); /* There must be at least one stack segment. Therefore it is a fatal error if "trailer" is null. */ if (trailer == 0) abort (); /* Discard segments that do not contain our argument address. */ while (trailer != 0) { block = (long *) trailer->this_address; size = trailer->this_size; if (block == 0 || size == 0) abort (); trailer = (struct stk_trailer *) trailer->link; if ((block <= address) && (address < (block + size))) break; } /* Set the result to the offset in this segment and add the sizes of all predecessor segments. */ result = address - block; if (trailer == 0) { return result; } do { if (trailer->this_size <= 0) abort (); result += trailer->this_size; trailer = (struct stk_trailer *) trailer->link; } while (trailer != 0); /* We are done. Note that if you present a bogus address (one not in any segment), you will get a different number back, formed from subtracting the address of the first block. This is probably not what you want. */ return (result); } # else /* not CRAY2 */ /* Stack address function for a CRAY-1, CRAY X-MP, or CRAY Y-MP. Determine the number of the cell within the stack, given the address of the cell. The purpose of this routine is to linearize, in some sense, stack addresses for alloca. */ static long i00afunc (long address) { long stkl = 0; long size, pseg, this_segment, stack; long result = 0; struct stack_segment_linkage *ssptr; /* Register B67 contains the address of the end of the current stack segment. If you (as a subprogram) store your registers on the stack and find that you are past the contents of B67, you have overflowed the segment. B67 also points to the stack segment linkage control area, which is what we are really interested in. */ stkl = CRAY_STACKSEG_END (); ssptr = (struct stack_segment_linkage *) stkl; /* If one subtracts 'size' from the end of the segment, one has the address of the first word of the segment. If this is not the first segment, 'pseg' will be nonzero. */ pseg = ssptr->sspseg; size = ssptr->sssize; this_segment = stkl - size; /* It is possible that calling this routine itself caused a stack overflow. Discard stack segments which do not contain the target address. */ while (!(this_segment <= address && address <= stkl)) { # ifdef DEBUG_I00AFUNC fprintf (stderr, "%011o %011o %011o\n", this_segment, address, stkl); # endif if (pseg == 0) break; stkl = stkl - pseg; ssptr = (struct stack_segment_linkage *) stkl; size = ssptr->sssize; pseg = ssptr->sspseg; this_segment = stkl - size; } result = address - this_segment; /* If you subtract pseg from the current end of the stack, you get the address of the previous stack segment's end. This seems a little convoluted to me, but I'll bet you save a cycle somewhere. */ while (pseg != 0) { # ifdef DEBUG_I00AFUNC fprintf (stderr, "%011o %011o\n", pseg, size); # endif stkl = stkl - pseg; ssptr = (struct stack_segment_linkage *) stkl; size = ssptr->sssize; pseg = ssptr->sspseg; result += size; } return (result); } # endif /* not CRAY2 */ # endif /* CRAY */ # endif /* no alloca */ #endif /* not GCC 2 */ gnuastro-0.2.33-8a3b/bootstrapped/lib/Makefile.in0000644000175000017500000043225513004464627016457 00000000000000# Makefile.in generated by automake 1.15 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2014 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY, to the extent permitted by law; without # even the implied warranty of MERCHANTABILITY or FITNESS FOR A # PARTICULAR PURPOSE. @SET_MAKE@ # Copyright (C) 2002-2016 Free Software Foundation, Inc. # # This file is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This file is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. 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@GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ REPLACE_READ = @REPLACE_READ@ REPLACE_READLINK = @REPLACE_READLINK@ REPLACE_READLINKAT = @REPLACE_READLINKAT@ REPLACE_REALLOC = @REPLACE_REALLOC@ REPLACE_REALPATH = @REPLACE_REALPATH@ REPLACE_REMAINDER = @REPLACE_REMAINDER@ REPLACE_REMAINDERF = @REPLACE_REMAINDERF@ REPLACE_REMAINDERL = @REPLACE_REMAINDERL@ REPLACE_REMOVE = @REPLACE_REMOVE@ REPLACE_RENAME = @REPLACE_RENAME@ REPLACE_RENAMEAT = @REPLACE_RENAMEAT@ REPLACE_RMDIR = @REPLACE_RMDIR@ REPLACE_ROUND = @REPLACE_ROUND@ REPLACE_ROUNDF = @REPLACE_ROUNDF@ REPLACE_ROUNDL = @REPLACE_ROUNDL@ REPLACE_SETENV = @REPLACE_SETENV@ REPLACE_SETLOCALE = @REPLACE_SETLOCALE@ REPLACE_SIGNBIT = @REPLACE_SIGNBIT@ REPLACE_SIGNBIT_USING_GCC = @REPLACE_SIGNBIT_USING_GCC@ REPLACE_SLEEP = @REPLACE_SLEEP@ REPLACE_SNPRINTF = @REPLACE_SNPRINTF@ REPLACE_SPRINTF = @REPLACE_SPRINTF@ REPLACE_SQRTL = @REPLACE_SQRTL@ REPLACE_STAT = @REPLACE_STAT@ REPLACE_STDIO_READ_FUNCS = @REPLACE_STDIO_READ_FUNCS@ REPLACE_STDIO_WRITE_FUNCS = @REPLACE_STDIO_WRITE_FUNCS@ REPLACE_STPNCPY = @REPLACE_STPNCPY@ REPLACE_STRCASESTR = @REPLACE_STRCASESTR@ REPLACE_STRCHRNUL = @REPLACE_STRCHRNUL@ REPLACE_STRDUP = @REPLACE_STRDUP@ REPLACE_STRERROR = @REPLACE_STRERROR@ REPLACE_STRERROR_R = 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GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT_AS_FIRST_DIRECTIVE''@|$(INCLUDE_NEXT_AS_FIRST_DIRECTIVE)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_AS_FIRST_DIRECTIVE_MATH_H''@|$(NEXT_AS_FIRST_DIRECTIVE_MATH_H)|g' \ -e 's/@''GNULIB_ACOSF''@/$(GNULIB_ACOSF)/g' \ -e 's/@''GNULIB_ACOSL''@/$(GNULIB_ACOSL)/g' \ -e 's/@''GNULIB_ASINF''@/$(GNULIB_ASINF)/g' \ -e 's/@''GNULIB_ASINL''@/$(GNULIB_ASINL)/g' \ -e 's/@''GNULIB_ATANF''@/$(GNULIB_ATANF)/g' \ -e 's/@''GNULIB_ATANL''@/$(GNULIB_ATANL)/g' \ -e 's/@''GNULIB_ATAN2F''@/$(GNULIB_ATAN2F)/g' \ -e 's/@''GNULIB_CBRT''@/$(GNULIB_CBRT)/g' \ -e 's/@''GNULIB_CBRTF''@/$(GNULIB_CBRTF)/g' \ -e 's/@''GNULIB_CBRTL''@/$(GNULIB_CBRTL)/g' \ -e 's/@''GNULIB_CEIL''@/$(GNULIB_CEIL)/g' \ -e 's/@''GNULIB_CEILF''@/$(GNULIB_CEILF)/g' \ -e 's/@''GNULIB_CEILL''@/$(GNULIB_CEILL)/g' \ -e 's/@''GNULIB_COPYSIGN''@/$(GNULIB_COPYSIGN)/g' \ -e 's/@''GNULIB_COPYSIGNF''@/$(GNULIB_COPYSIGNF)/g' \ -e 's/@''GNULIB_COPYSIGNL''@/$(GNULIB_COPYSIGNL)/g' \ -e 's/@''GNULIB_COSF''@/$(GNULIB_COSF)/g' \ -e 's/@''GNULIB_COSL''@/$(GNULIB_COSL)/g' \ -e 's/@''GNULIB_COSHF''@/$(GNULIB_COSHF)/g' \ -e 's/@''GNULIB_EXPF''@/$(GNULIB_EXPF)/g' \ -e 's/@''GNULIB_EXPL''@/$(GNULIB_EXPL)/g' \ -e 's/@''GNULIB_EXP2''@/$(GNULIB_EXP2)/g' \ -e 's/@''GNULIB_EXP2F''@/$(GNULIB_EXP2F)/g' \ -e 's/@''GNULIB_EXP2L''@/$(GNULIB_EXP2L)/g' \ -e 's/@''GNULIB_EXPM1''@/$(GNULIB_EXPM1)/g' \ -e 's/@''GNULIB_EXPM1F''@/$(GNULIB_EXPM1F)/g' \ -e 's/@''GNULIB_EXPM1L''@/$(GNULIB_EXPM1L)/g' \ -e 's/@''GNULIB_FABSF''@/$(GNULIB_FABSF)/g' \ -e 's/@''GNULIB_FABSL''@/$(GNULIB_FABSL)/g' \ -e 's/@''GNULIB_FLOOR''@/$(GNULIB_FLOOR)/g' \ -e 's/@''GNULIB_FLOORF''@/$(GNULIB_FLOORF)/g' \ -e 's/@''GNULIB_FLOORL''@/$(GNULIB_FLOORL)/g' \ -e 's/@''GNULIB_FMA''@/$(GNULIB_FMA)/g' \ -e 's/@''GNULIB_FMAF''@/$(GNULIB_FMAF)/g' \ -e 's/@''GNULIB_FMAL''@/$(GNULIB_FMAL)/g' \ -e 's/@''GNULIB_FMOD''@/$(GNULIB_FMOD)/g' \ -e 's/@''GNULIB_FMODF''@/$(GNULIB_FMODF)/g' \ -e 's/@''GNULIB_FMODL''@/$(GNULIB_FMODL)/g' \ -e 's/@''GNULIB_FREXPF''@/$(GNULIB_FREXPF)/g' \ -e 's/@''GNULIB_FREXP''@/$(GNULIB_FREXP)/g' \ -e 's/@''GNULIB_FREXPL''@/$(GNULIB_FREXPL)/g' \ -e 's/@''GNULIB_HYPOT''@/$(GNULIB_HYPOT)/g' \ -e 's/@''GNULIB_HYPOTF''@/$(GNULIB_HYPOTF)/g' \ -e 's/@''GNULIB_HYPOTL''@/$(GNULIB_HYPOTL)/g' \ < $(srcdir)/math.in.h | \ sed -e 's/@''GNULIB_ILOGB''@/$(GNULIB_ILOGB)/g' \ -e 's/@''GNULIB_ILOGBF''@/$(GNULIB_ILOGBF)/g' \ -e 's/@''GNULIB_ILOGBL''@/$(GNULIB_ILOGBL)/g' \ -e 's/@''GNULIB_ISFINITE''@/$(GNULIB_ISFINITE)/g' \ -e 's/@''GNULIB_ISINF''@/$(GNULIB_ISINF)/g' \ -e 's/@''GNULIB_ISNAN''@/$(GNULIB_ISNAN)/g' \ -e 's/@''GNULIB_ISNANF''@/$(GNULIB_ISNANF)/g' \ -e 's/@''GNULIB_ISNAND''@/$(GNULIB_ISNAND)/g' \ -e 's/@''GNULIB_ISNANL''@/$(GNULIB_ISNANL)/g' \ -e 's/@''GNULIB_LDEXPF''@/$(GNULIB_LDEXPF)/g' \ -e 's/@''GNULIB_LDEXPL''@/$(GNULIB_LDEXPL)/g' \ -e 's/@''GNULIB_LOG''@/$(GNULIB_LOG)/g' \ -e 's/@''GNULIB_LOGF''@/$(GNULIB_LOGF)/g' \ -e 's/@''GNULIB_LOGL''@/$(GNULIB_LOGL)/g' \ -e 's/@''GNULIB_LOG10''@/$(GNULIB_LOG10)/g' \ -e 's/@''GNULIB_LOG10F''@/$(GNULIB_LOG10F)/g' \ -e 's/@''GNULIB_LOG10L''@/$(GNULIB_LOG10L)/g' \ -e 's/@''GNULIB_LOG1P''@/$(GNULIB_LOG1P)/g' \ -e 's/@''GNULIB_LOG1PF''@/$(GNULIB_LOG1PF)/g' \ -e 's/@''GNULIB_LOG1PL''@/$(GNULIB_LOG1PL)/g' \ -e 's/@''GNULIB_LOG2''@/$(GNULIB_LOG2)/g' \ -e 's/@''GNULIB_LOG2F''@/$(GNULIB_LOG2F)/g' \ -e 's/@''GNULIB_LOG2L''@/$(GNULIB_LOG2L)/g' \ -e 's/@''GNULIB_LOGB''@/$(GNULIB_LOGB)/g' \ -e 's/@''GNULIB_LOGBF''@/$(GNULIB_LOGBF)/g' \ -e 's/@''GNULIB_LOGBL''@/$(GNULIB_LOGBL)/g' \ -e 's/@''GNULIB_MODF''@/$(GNULIB_MODF)/g' \ -e 's/@''GNULIB_MODFF''@/$(GNULIB_MODFF)/g' \ -e 's/@''GNULIB_MODFL''@/$(GNULIB_MODFL)/g' \ -e 's/@''GNULIB_POWF''@/$(GNULIB_POWF)/g' \ -e 's/@''GNULIB_REMAINDER''@/$(GNULIB_REMAINDER)/g' \ -e 's/@''GNULIB_REMAINDERF''@/$(GNULIB_REMAINDERF)/g' \ -e 's/@''GNULIB_REMAINDERL''@/$(GNULIB_REMAINDERL)/g' \ -e 's/@''GNULIB_RINT''@/$(GNULIB_RINT)/g' \ -e 's/@''GNULIB_RINTF''@/$(GNULIB_RINTF)/g' \ -e 's/@''GNULIB_RINTL''@/$(GNULIB_RINTL)/g' \ -e 's/@''GNULIB_ROUND''@/$(GNULIB_ROUND)/g' \ -e 's/@''GNULIB_ROUNDF''@/$(GNULIB_ROUNDF)/g' \ -e 's/@''GNULIB_ROUNDL''@/$(GNULIB_ROUNDL)/g' \ -e 's/@''GNULIB_SIGNBIT''@/$(GNULIB_SIGNBIT)/g' \ -e 's/@''GNULIB_SINF''@/$(GNULIB_SINF)/g' \ -e 's/@''GNULIB_SINL''@/$(GNULIB_SINL)/g' \ -e 's/@''GNULIB_SINHF''@/$(GNULIB_SINHF)/g' \ -e 's/@''GNULIB_SQRTF''@/$(GNULIB_SQRTF)/g' \ -e 's/@''GNULIB_SQRTL''@/$(GNULIB_SQRTL)/g' \ -e 's/@''GNULIB_TANF''@/$(GNULIB_TANF)/g' \ -e 's/@''GNULIB_TANL''@/$(GNULIB_TANL)/g' \ -e 's/@''GNULIB_TANHF''@/$(GNULIB_TANHF)/g' \ -e 's/@''GNULIB_TRUNC''@/$(GNULIB_TRUNC)/g' \ -e 's/@''GNULIB_TRUNCF''@/$(GNULIB_TRUNCF)/g' \ -e 's/@''GNULIB_TRUNCL''@/$(GNULIB_TRUNCL)/g' \ | \ sed -e 's|@''HAVE_ACOSF''@|$(HAVE_ACOSF)|g' \ -e 's|@''HAVE_ACOSL''@|$(HAVE_ACOSL)|g' \ -e 's|@''HAVE_ASINF''@|$(HAVE_ASINF)|g' \ -e 's|@''HAVE_ASINL''@|$(HAVE_ASINL)|g' \ -e 's|@''HAVE_ATANF''@|$(HAVE_ATANF)|g' \ -e 's|@''HAVE_ATANL''@|$(HAVE_ATANL)|g' \ -e 's|@''HAVE_ATAN2F''@|$(HAVE_ATAN2F)|g' \ -e 's|@''HAVE_CBRT''@|$(HAVE_CBRT)|g' \ -e 's|@''HAVE_CBRTF''@|$(HAVE_CBRTF)|g' \ -e 's|@''HAVE_CBRTL''@|$(HAVE_CBRTL)|g' \ -e 's|@''HAVE_COPYSIGN''@|$(HAVE_COPYSIGN)|g' \ -e 's|@''HAVE_COPYSIGNL''@|$(HAVE_COPYSIGNL)|g' \ -e 's|@''HAVE_COSF''@|$(HAVE_COSF)|g' \ -e 's|@''HAVE_COSL''@|$(HAVE_COSL)|g' \ -e 's|@''HAVE_COSHF''@|$(HAVE_COSHF)|g' \ -e 's|@''HAVE_EXPF''@|$(HAVE_EXPF)|g' \ -e 's|@''HAVE_EXPL''@|$(HAVE_EXPL)|g' \ -e 's|@''HAVE_EXPM1''@|$(HAVE_EXPM1)|g' \ -e 's|@''HAVE_EXPM1F''@|$(HAVE_EXPM1F)|g' \ -e 's|@''HAVE_FABSF''@|$(HAVE_FABSF)|g' \ -e 's|@''HAVE_FABSL''@|$(HAVE_FABSL)|g' \ -e 's|@''HAVE_FMA''@|$(HAVE_FMA)|g' \ -e 's|@''HAVE_FMAF''@|$(HAVE_FMAF)|g' \ -e 's|@''HAVE_FMAL''@|$(HAVE_FMAL)|g' \ -e 's|@''HAVE_FMODF''@|$(HAVE_FMODF)|g' \ -e 's|@''HAVE_FMODL''@|$(HAVE_FMODL)|g' \ -e 's|@''HAVE_FREXPF''@|$(HAVE_FREXPF)|g' \ -e 's|@''HAVE_HYPOTF''@|$(HAVE_HYPOTF)|g' \ -e 's|@''HAVE_HYPOTL''@|$(HAVE_HYPOTL)|g' \ -e 's|@''HAVE_ILOGB''@|$(HAVE_ILOGB)|g' \ -e 's|@''HAVE_ILOGBF''@|$(HAVE_ILOGBF)|g' \ -e 's|@''HAVE_ILOGBL''@|$(HAVE_ILOGBL)|g' \ -e 's|@''HAVE_ISNANF''@|$(HAVE_ISNANF)|g' \ -e 's|@''HAVE_ISNAND''@|$(HAVE_ISNAND)|g' \ -e 's|@''HAVE_ISNANL''@|$(HAVE_ISNANL)|g' \ -e 's|@''HAVE_LDEXPF''@|$(HAVE_LDEXPF)|g' \ -e 's|@''HAVE_LOGF''@|$(HAVE_LOGF)|g' \ -e 's|@''HAVE_LOGL''@|$(HAVE_LOGL)|g' \ -e 's|@''HAVE_LOG10F''@|$(HAVE_LOG10F)|g' \ -e 's|@''HAVE_LOG10L''@|$(HAVE_LOG10L)|g' \ -e 's|@''HAVE_LOG1P''@|$(HAVE_LOG1P)|g' \ -e 's|@''HAVE_LOG1PF''@|$(HAVE_LOG1PF)|g' \ -e 's|@''HAVE_LOG1PL''@|$(HAVE_LOG1PL)|g' \ -e 's|@''HAVE_LOGBF''@|$(HAVE_LOGBF)|g' \ -e 's|@''HAVE_LOGBL''@|$(HAVE_LOGBL)|g' \ -e 's|@''HAVE_MODFF''@|$(HAVE_MODFF)|g' \ -e 's|@''HAVE_MODFL''@|$(HAVE_MODFL)|g' \ -e 's|@''HAVE_POWF''@|$(HAVE_POWF)|g' \ -e 's|@''HAVE_REMAINDER''@|$(HAVE_REMAINDER)|g' \ -e 's|@''HAVE_REMAINDERF''@|$(HAVE_REMAINDERF)|g' \ -e 's|@''HAVE_RINT''@|$(HAVE_RINT)|g' \ -e 's|@''HAVE_RINTL''@|$(HAVE_RINTL)|g' \ -e 's|@''HAVE_SINF''@|$(HAVE_SINF)|g' \ -e 's|@''HAVE_SINL''@|$(HAVE_SINL)|g' \ -e 's|@''HAVE_SINHF''@|$(HAVE_SINHF)|g' \ -e 's|@''HAVE_SQRTF''@|$(HAVE_SQRTF)|g' \ -e 's|@''HAVE_SQRTL''@|$(HAVE_SQRTL)|g' \ -e 's|@''HAVE_TANF''@|$(HAVE_TANF)|g' \ -e 's|@''HAVE_TANL''@|$(HAVE_TANL)|g' \ -e 's|@''HAVE_TANHF''@|$(HAVE_TANHF)|g' \ -e 's|@''HAVE_DECL_ACOSL''@|$(HAVE_DECL_ACOSL)|g' \ -e 's|@''HAVE_DECL_ASINL''@|$(HAVE_DECL_ASINL)|g' \ -e 's|@''HAVE_DECL_ATANL''@|$(HAVE_DECL_ATANL)|g' \ -e 's|@''HAVE_DECL_CBRTF''@|$(HAVE_DECL_CBRTF)|g' \ -e 's|@''HAVE_DECL_CBRTL''@|$(HAVE_DECL_CBRTL)|g' \ -e 's|@''HAVE_DECL_CEILF''@|$(HAVE_DECL_CEILF)|g' \ -e 's|@''HAVE_DECL_CEILL''@|$(HAVE_DECL_CEILL)|g' \ -e 's|@''HAVE_DECL_COPYSIGNF''@|$(HAVE_DECL_COPYSIGNF)|g' \ -e 's|@''HAVE_DECL_COSL''@|$(HAVE_DECL_COSL)|g' \ -e 's|@''HAVE_DECL_EXPL''@|$(HAVE_DECL_EXPL)|g' \ -e 's|@''HAVE_DECL_EXP2''@|$(HAVE_DECL_EXP2)|g' \ -e 's|@''HAVE_DECL_EXP2F''@|$(HAVE_DECL_EXP2F)|g' \ -e 's|@''HAVE_DECL_EXP2L''@|$(HAVE_DECL_EXP2L)|g' \ -e 's|@''HAVE_DECL_EXPM1L''@|$(HAVE_DECL_EXPM1L)|g' \ -e 's|@''HAVE_DECL_FLOORF''@|$(HAVE_DECL_FLOORF)|g' \ -e 's|@''HAVE_DECL_FLOORL''@|$(HAVE_DECL_FLOORL)|g' \ -e 's|@''HAVE_DECL_FREXPL''@|$(HAVE_DECL_FREXPL)|g' \ -e 's|@''HAVE_DECL_LDEXPL''@|$(HAVE_DECL_LDEXPL)|g' \ -e 's|@''HAVE_DECL_LOGL''@|$(HAVE_DECL_LOGL)|g' \ -e 's|@''HAVE_DECL_LOG10L''@|$(HAVE_DECL_LOG10L)|g' \ -e 's|@''HAVE_DECL_LOG2''@|$(HAVE_DECL_LOG2)|g' \ -e 's|@''HAVE_DECL_LOG2F''@|$(HAVE_DECL_LOG2F)|g' \ -e 's|@''HAVE_DECL_LOG2L''@|$(HAVE_DECL_LOG2L)|g' \ -e 's|@''HAVE_DECL_LOGB''@|$(HAVE_DECL_LOGB)|g' \ -e 's|@''HAVE_DECL_REMAINDER''@|$(HAVE_DECL_REMAINDER)|g' \ -e 's|@''HAVE_DECL_REMAINDERL''@|$(HAVE_DECL_REMAINDERL)|g' \ -e 's|@''HAVE_DECL_RINTF''@|$(HAVE_DECL_RINTF)|g' \ -e 's|@''HAVE_DECL_ROUND''@|$(HAVE_DECL_ROUND)|g' \ -e 's|@''HAVE_DECL_ROUNDF''@|$(HAVE_DECL_ROUNDF)|g' \ -e 's|@''HAVE_DECL_ROUNDL''@|$(HAVE_DECL_ROUNDL)|g' \ -e 's|@''HAVE_DECL_SINL''@|$(HAVE_DECL_SINL)|g' \ -e 's|@''HAVE_DECL_SQRTL''@|$(HAVE_DECL_SQRTL)|g' \ -e 's|@''HAVE_DECL_TANL''@|$(HAVE_DECL_TANL)|g' \ -e 's|@''HAVE_DECL_TRUNC''@|$(HAVE_DECL_TRUNC)|g' \ -e 's|@''HAVE_DECL_TRUNCF''@|$(HAVE_DECL_TRUNCF)|g' \ -e 's|@''HAVE_DECL_TRUNCL''@|$(HAVE_DECL_TRUNCL)|g' \ | \ sed -e 's|@''REPLACE_CBRTF''@|$(REPLACE_CBRTF)|g' \ -e 's|@''REPLACE_CBRTL''@|$(REPLACE_CBRTL)|g' \ -e 's|@''REPLACE_CEIL''@|$(REPLACE_CEIL)|g' \ -e 's|@''REPLACE_CEILF''@|$(REPLACE_CEILF)|g' \ -e 's|@''REPLACE_CEILL''@|$(REPLACE_CEILL)|g' \ -e 's|@''REPLACE_EXPM1''@|$(REPLACE_EXPM1)|g' \ -e 's|@''REPLACE_EXPM1F''@|$(REPLACE_EXPM1F)|g' \ -e 's|@''REPLACE_EXP2''@|$(REPLACE_EXP2)|g' \ -e 's|@''REPLACE_EXP2L''@|$(REPLACE_EXP2L)|g' \ -e 's|@''REPLACE_FABSL''@|$(REPLACE_FABSL)|g' \ -e 's|@''REPLACE_FLOOR''@|$(REPLACE_FLOOR)|g' \ -e 's|@''REPLACE_FLOORF''@|$(REPLACE_FLOORF)|g' \ -e 's|@''REPLACE_FLOORL''@|$(REPLACE_FLOORL)|g' \ -e 's|@''REPLACE_FMA''@|$(REPLACE_FMA)|g' \ -e 's|@''REPLACE_FMAF''@|$(REPLACE_FMAF)|g' \ -e 's|@''REPLACE_FMAL''@|$(REPLACE_FMAL)|g' \ -e 's|@''REPLACE_FMOD''@|$(REPLACE_FMOD)|g' \ -e 's|@''REPLACE_FMODF''@|$(REPLACE_FMODF)|g' \ -e 's|@''REPLACE_FMODL''@|$(REPLACE_FMODL)|g' \ -e 's|@''REPLACE_FREXPF''@|$(REPLACE_FREXPF)|g' \ -e 's|@''REPLACE_FREXP''@|$(REPLACE_FREXP)|g' \ -e 's|@''REPLACE_FREXPL''@|$(REPLACE_FREXPL)|g' \ -e 's|@''REPLACE_HUGE_VAL''@|$(REPLACE_HUGE_VAL)|g' \ -e 's|@''REPLACE_HYPOT''@|$(REPLACE_HYPOT)|g' \ -e 's|@''REPLACE_HYPOTF''@|$(REPLACE_HYPOTF)|g' \ -e 's|@''REPLACE_HYPOTL''@|$(REPLACE_HYPOTL)|g' \ -e 's|@''REPLACE_ILOGB''@|$(REPLACE_ILOGB)|g' \ -e 's|@''REPLACE_ILOGBF''@|$(REPLACE_ILOGBF)|g' \ -e 's|@''REPLACE_ISFINITE''@|$(REPLACE_ISFINITE)|g' \ -e 's|@''REPLACE_ISINF''@|$(REPLACE_ISINF)|g' \ -e 's|@''REPLACE_ISNAN''@|$(REPLACE_ISNAN)|g' \ -e 's|@''REPLACE_ITOLD''@|$(REPLACE_ITOLD)|g' \ -e 's|@''REPLACE_LDEXPL''@|$(REPLACE_LDEXPL)|g' \ -e 's|@''REPLACE_LOG''@|$(REPLACE_LOG)|g' \ -e 's|@''REPLACE_LOGF''@|$(REPLACE_LOGF)|g' \ -e 's|@''REPLACE_LOGL''@|$(REPLACE_LOGL)|g' \ -e 's|@''REPLACE_LOG10''@|$(REPLACE_LOG10)|g' \ -e 's|@''REPLACE_LOG10F''@|$(REPLACE_LOG10F)|g' \ -e 's|@''REPLACE_LOG10L''@|$(REPLACE_LOG10L)|g' \ -e 's|@''REPLACE_LOG1P''@|$(REPLACE_LOG1P)|g' \ -e 's|@''REPLACE_LOG1PF''@|$(REPLACE_LOG1PF)|g' \ -e 's|@''REPLACE_LOG1PL''@|$(REPLACE_LOG1PL)|g' \ -e 's|@''REPLACE_LOG2''@|$(REPLACE_LOG2)|g' \ -e 's|@''REPLACE_LOG2F''@|$(REPLACE_LOG2F)|g' \ -e 's|@''REPLACE_LOG2L''@|$(REPLACE_LOG2L)|g' \ -e 's|@''REPLACE_LOGB''@|$(REPLACE_LOGB)|g' \ -e 's|@''REPLACE_LOGBF''@|$(REPLACE_LOGBF)|g' \ -e 's|@''REPLACE_LOGBL''@|$(REPLACE_LOGBL)|g' \ -e 's|@''REPLACE_MODF''@|$(REPLACE_MODF)|g' \ -e 's|@''REPLACE_MODFF''@|$(REPLACE_MODFF)|g' \ -e 's|@''REPLACE_MODFL''@|$(REPLACE_MODFL)|g' \ -e 's|@''REPLACE_NAN''@|$(REPLACE_NAN)|g' \ -e 's|@''REPLACE_REMAINDER''@|$(REPLACE_REMAINDER)|g' \ -e 's|@''REPLACE_REMAINDERF''@|$(REPLACE_REMAINDERF)|g' \ -e 's|@''REPLACE_REMAINDERL''@|$(REPLACE_REMAINDERL)|g' \ -e 's|@''REPLACE_ROUND''@|$(REPLACE_ROUND)|g' \ -e 's|@''REPLACE_ROUNDF''@|$(REPLACE_ROUNDF)|g' \ -e 's|@''REPLACE_ROUNDL''@|$(REPLACE_ROUNDL)|g' \ -e 's|@''REPLACE_SIGNBIT''@|$(REPLACE_SIGNBIT)|g' \ -e 's|@''REPLACE_SIGNBIT_USING_GCC''@|$(REPLACE_SIGNBIT_USING_GCC)|g' \ -e 's|@''REPLACE_SQRTL''@|$(REPLACE_SQRTL)|g' \ -e 's|@''REPLACE_TRUNC''@|$(REPLACE_TRUNC)|g' \ -e 's|@''REPLACE_TRUNCF''@|$(REPLACE_TRUNCF)|g' \ -e 's|@''REPLACE_TRUNCL''@|$(REPLACE_TRUNCL)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ # The arg-nonnull.h that gets inserted into generated .h files is the same as # build-aux/snippet/arg-nonnull.h, except that it has the copyright header cut # off. arg-nonnull.h: $(top_srcdir)/bootstrapped/build-aux/snippet/arg-nonnull.h $(AM_V_GEN)rm -f $@-t $@ && \ sed -n -e '/GL_ARG_NONNULL/,$$p' \ < $(top_srcdir)/bootstrapped/build-aux/snippet/arg-nonnull.h \ > $@-t && \ mv $@-t $@ # The c++defs.h that gets inserted into generated .h files is the same as # build-aux/snippet/c++defs.h, except that it has the copyright header cut off. c++defs.h: $(top_srcdir)/bootstrapped/build-aux/snippet/c++defs.h $(AM_V_GEN)rm -f $@-t $@ && \ sed -n -e '/_GL_CXXDEFS/,$$p' \ < $(top_srcdir)/bootstrapped/build-aux/snippet/c++defs.h \ > $@-t && \ mv $@-t $@ # The warn-on-use.h that gets inserted into generated .h files is the same as # build-aux/snippet/warn-on-use.h, except that it has the copyright header cut # off. warn-on-use.h: $(top_srcdir)/bootstrapped/build-aux/snippet/warn-on-use.h $(AM_V_GEN)rm -f $@-t $@ && \ sed -n -e '/^.ifndef/,$$p' \ < $(top_srcdir)/bootstrapped/build-aux/snippet/warn-on-use.h \ > $@-t && \ mv $@-t $@ # We need the following in order to create when the system # doesn't have one that works. @GL_GENERATE_STDALIGN_H_TRUE@stdalign.h: stdalign.in.h $(top_builddir)/config.status @GL_GENERATE_STDALIGN_H_TRUE@ $(AM_V_GEN)rm -f $@-t $@ && \ @GL_GENERATE_STDALIGN_H_TRUE@ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ @GL_GENERATE_STDALIGN_H_TRUE@ cat $(srcdir)/stdalign.in.h; \ @GL_GENERATE_STDALIGN_H_TRUE@ } > $@-t && \ @GL_GENERATE_STDALIGN_H_TRUE@ mv $@-t $@ @GL_GENERATE_STDALIGN_H_FALSE@stdalign.h: $(top_builddir)/config.status @GL_GENERATE_STDALIGN_H_FALSE@ rm -f $@ # We need the following in order to create when the system # doesn't have one that works. @GL_GENERATE_STDBOOL_H_TRUE@stdbool.h: stdbool.in.h $(top_builddir)/config.status @GL_GENERATE_STDBOOL_H_TRUE@ $(AM_V_GEN)rm -f $@-t $@ && \ @GL_GENERATE_STDBOOL_H_TRUE@ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ @GL_GENERATE_STDBOOL_H_TRUE@ sed -e 's/@''HAVE__BOOL''@/$(HAVE__BOOL)/g' < $(srcdir)/stdbool.in.h; \ @GL_GENERATE_STDBOOL_H_TRUE@ } > $@-t && \ @GL_GENERATE_STDBOOL_H_TRUE@ mv $@-t $@ @GL_GENERATE_STDBOOL_H_FALSE@stdbool.h: $(top_builddir)/config.status @GL_GENERATE_STDBOOL_H_FALSE@ rm -f $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. @GL_GENERATE_STDDEF_H_TRUE@stddef.h: stddef.in.h $(top_builddir)/config.status @GL_GENERATE_STDDEF_H_TRUE@ $(AM_V_GEN)rm -f $@-t $@ && \ @GL_GENERATE_STDDEF_H_TRUE@ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ @GL_GENERATE_STDDEF_H_TRUE@ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ @GL_GENERATE_STDDEF_H_TRUE@ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ @GL_GENERATE_STDDEF_H_TRUE@ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ @GL_GENERATE_STDDEF_H_TRUE@ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ @GL_GENERATE_STDDEF_H_TRUE@ -e 's|@''NEXT_STDDEF_H''@|$(NEXT_STDDEF_H)|g' \ @GL_GENERATE_STDDEF_H_TRUE@ -e 's|@''HAVE_MAX_ALIGN_T''@|$(HAVE_MAX_ALIGN_T)|g' \ @GL_GENERATE_STDDEF_H_TRUE@ -e 's|@''HAVE_WCHAR_T''@|$(HAVE_WCHAR_T)|g' \ @GL_GENERATE_STDDEF_H_TRUE@ -e 's|@''REPLACE_NULL''@|$(REPLACE_NULL)|g' \ @GL_GENERATE_STDDEF_H_TRUE@ < $(srcdir)/stddef.in.h; \ @GL_GENERATE_STDDEF_H_TRUE@ } > $@-t && \ @GL_GENERATE_STDDEF_H_TRUE@ mv $@-t $@ @GL_GENERATE_STDDEF_H_FALSE@stddef.h: $(top_builddir)/config.status @GL_GENERATE_STDDEF_H_FALSE@ rm -f $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. @GL_GENERATE_STDINT_H_TRUE@stdint.h: stdint.in.h $(top_builddir)/config.status @GL_GENERATE_STDINT_H_TRUE@ $(AM_V_GEN)rm -f $@-t $@ && \ @GL_GENERATE_STDINT_H_TRUE@ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ @GL_GENERATE_STDINT_H_TRUE@ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_STDINT_H''@/$(HAVE_STDINT_H)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's|@''NEXT_STDINT_H''@|$(NEXT_STDINT_H)|g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_C99_STDINT_H''@/$(HAVE_C99_STDINT_H)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_SYS_TYPES_H''@/$(HAVE_SYS_TYPES_H)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_INTTYPES_H''@/$(HAVE_INTTYPES_H)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_SYS_INTTYPES_H''@/$(HAVE_SYS_INTTYPES_H)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_SYS_BITYPES_H''@/$(HAVE_SYS_BITYPES_H)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_WCHAR_H''@/$(HAVE_WCHAR_H)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_LONG_LONG_INT''@/$(HAVE_LONG_LONG_INT)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_UNSIGNED_LONG_LONG_INT''@/$(HAVE_UNSIGNED_LONG_LONG_INT)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''APPLE_UNIVERSAL_BUILD''@/$(APPLE_UNIVERSAL_BUILD)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''BITSIZEOF_PTRDIFF_T''@/$(BITSIZEOF_PTRDIFF_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''PTRDIFF_T_SUFFIX''@/$(PTRDIFF_T_SUFFIX)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''BITSIZEOF_SIG_ATOMIC_T''@/$(BITSIZEOF_SIG_ATOMIC_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_SIGNED_SIG_ATOMIC_T''@/$(HAVE_SIGNED_SIG_ATOMIC_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''SIG_ATOMIC_T_SUFFIX''@/$(SIG_ATOMIC_T_SUFFIX)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''BITSIZEOF_SIZE_T''@/$(BITSIZEOF_SIZE_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''SIZE_T_SUFFIX''@/$(SIZE_T_SUFFIX)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''BITSIZEOF_WCHAR_T''@/$(BITSIZEOF_WCHAR_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_SIGNED_WCHAR_T''@/$(HAVE_SIGNED_WCHAR_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''WCHAR_T_SUFFIX''@/$(WCHAR_T_SUFFIX)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''BITSIZEOF_WINT_T''@/$(BITSIZEOF_WINT_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_SIGNED_WINT_T''@/$(HAVE_SIGNED_WINT_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''WINT_T_SUFFIX''@/$(WINT_T_SUFFIX)/g' \ @GL_GENERATE_STDINT_H_TRUE@ < $(srcdir)/stdint.in.h; \ @GL_GENERATE_STDINT_H_TRUE@ } > $@-t && \ @GL_GENERATE_STDINT_H_TRUE@ mv $@-t $@ @GL_GENERATE_STDINT_H_FALSE@stdint.h: $(top_builddir)/config.status @GL_GENERATE_STDINT_H_FALSE@ rm -f $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. stdio.h: stdio.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STDIO_H''@|$(NEXT_STDIO_H)|g' \ -e 's/@''GNULIB_DPRINTF''@/$(GNULIB_DPRINTF)/g' \ -e 's/@''GNULIB_FCLOSE''@/$(GNULIB_FCLOSE)/g' \ -e 's/@''GNULIB_FDOPEN''@/$(GNULIB_FDOPEN)/g' \ -e 's/@''GNULIB_FFLUSH''@/$(GNULIB_FFLUSH)/g' \ -e 's/@''GNULIB_FGETC''@/$(GNULIB_FGETC)/g' \ -e 's/@''GNULIB_FGETS''@/$(GNULIB_FGETS)/g' \ -e 's/@''GNULIB_FOPEN''@/$(GNULIB_FOPEN)/g' \ -e 's/@''GNULIB_FPRINTF''@/$(GNULIB_FPRINTF)/g' \ -e 's/@''GNULIB_FPRINTF_POSIX''@/$(GNULIB_FPRINTF_POSIX)/g' \ -e 's/@''GNULIB_FPURGE''@/$(GNULIB_FPURGE)/g' \ -e 's/@''GNULIB_FPUTC''@/$(GNULIB_FPUTC)/g' \ -e 's/@''GNULIB_FPUTS''@/$(GNULIB_FPUTS)/g' \ -e 's/@''GNULIB_FREAD''@/$(GNULIB_FREAD)/g' \ -e 's/@''GNULIB_FREOPEN''@/$(GNULIB_FREOPEN)/g' \ -e 's/@''GNULIB_FSCANF''@/$(GNULIB_FSCANF)/g' \ -e 's/@''GNULIB_FSEEK''@/$(GNULIB_FSEEK)/g' \ -e 's/@''GNULIB_FSEEKO''@/$(GNULIB_FSEEKO)/g' \ -e 's/@''GNULIB_FTELL''@/$(GNULIB_FTELL)/g' \ -e 's/@''GNULIB_FTELLO''@/$(GNULIB_FTELLO)/g' \ -e 's/@''GNULIB_FWRITE''@/$(GNULIB_FWRITE)/g' \ -e 's/@''GNULIB_GETC''@/$(GNULIB_GETC)/g' \ -e 's/@''GNULIB_GETCHAR''@/$(GNULIB_GETCHAR)/g' \ -e 's/@''GNULIB_GETDELIM''@/$(GNULIB_GETDELIM)/g' \ -e 's/@''GNULIB_GETLINE''@/$(GNULIB_GETLINE)/g' \ -e 's/@''GNULIB_OBSTACK_PRINTF''@/$(GNULIB_OBSTACK_PRINTF)/g' \ -e 's/@''GNULIB_OBSTACK_PRINTF_POSIX''@/$(GNULIB_OBSTACK_PRINTF_POSIX)/g' \ -e 's/@''GNULIB_PCLOSE''@/$(GNULIB_PCLOSE)/g' \ -e 's/@''GNULIB_PERROR''@/$(GNULIB_PERROR)/g' \ -e 's/@''GNULIB_POPEN''@/$(GNULIB_POPEN)/g' \ -e 's/@''GNULIB_PRINTF''@/$(GNULIB_PRINTF)/g' \ -e 's/@''GNULIB_PRINTF_POSIX''@/$(GNULIB_PRINTF_POSIX)/g' \ -e 's/@''GNULIB_PUTC''@/$(GNULIB_PUTC)/g' \ -e 's/@''GNULIB_PUTCHAR''@/$(GNULIB_PUTCHAR)/g' \ -e 's/@''GNULIB_PUTS''@/$(GNULIB_PUTS)/g' \ -e 's/@''GNULIB_REMOVE''@/$(GNULIB_REMOVE)/g' \ -e 's/@''GNULIB_RENAME''@/$(GNULIB_RENAME)/g' \ -e 's/@''GNULIB_RENAMEAT''@/$(GNULIB_RENAMEAT)/g' \ -e 's/@''GNULIB_SCANF''@/$(GNULIB_SCANF)/g' \ -e 's/@''GNULIB_SNPRINTF''@/$(GNULIB_SNPRINTF)/g' \ -e 's/@''GNULIB_SPRINTF_POSIX''@/$(GNULIB_SPRINTF_POSIX)/g' \ -e 's/@''GNULIB_STDIO_H_NONBLOCKING''@/$(GNULIB_STDIO_H_NONBLOCKING)/g' \ -e 's/@''GNULIB_STDIO_H_SIGPIPE''@/$(GNULIB_STDIO_H_SIGPIPE)/g' \ -e 's/@''GNULIB_TMPFILE''@/$(GNULIB_TMPFILE)/g' \ -e 's/@''GNULIB_VASPRINTF''@/$(GNULIB_VASPRINTF)/g' \ -e 's/@''GNULIB_VDPRINTF''@/$(GNULIB_VDPRINTF)/g' \ -e 's/@''GNULIB_VFPRINTF''@/$(GNULIB_VFPRINTF)/g' \ -e 's/@''GNULIB_VFPRINTF_POSIX''@/$(GNULIB_VFPRINTF_POSIX)/g' \ -e 's/@''GNULIB_VFSCANF''@/$(GNULIB_VFSCANF)/g' \ -e 's/@''GNULIB_VSCANF''@/$(GNULIB_VSCANF)/g' \ -e 's/@''GNULIB_VPRINTF''@/$(GNULIB_VPRINTF)/g' \ -e 's/@''GNULIB_VPRINTF_POSIX''@/$(GNULIB_VPRINTF_POSIX)/g' \ -e 's/@''GNULIB_VSNPRINTF''@/$(GNULIB_VSNPRINTF)/g' \ -e 's/@''GNULIB_VSPRINTF_POSIX''@/$(GNULIB_VSPRINTF_POSIX)/g' \ < $(srcdir)/stdio.in.h | \ sed -e 's|@''HAVE_DECL_FPURGE''@|$(HAVE_DECL_FPURGE)|g' \ -e 's|@''HAVE_DECL_FSEEKO''@|$(HAVE_DECL_FSEEKO)|g' \ -e 's|@''HAVE_DECL_FTELLO''@|$(HAVE_DECL_FTELLO)|g' \ -e 's|@''HAVE_DECL_GETDELIM''@|$(HAVE_DECL_GETDELIM)|g' \ -e 's|@''HAVE_DECL_GETLINE''@|$(HAVE_DECL_GETLINE)|g' \ -e 's|@''HAVE_DECL_OBSTACK_PRINTF''@|$(HAVE_DECL_OBSTACK_PRINTF)|g' \ -e 's|@''HAVE_DECL_SNPRINTF''@|$(HAVE_DECL_SNPRINTF)|g' \ -e 's|@''HAVE_DECL_VSNPRINTF''@|$(HAVE_DECL_VSNPRINTF)|g' \ -e 's|@''HAVE_DPRINTF''@|$(HAVE_DPRINTF)|g' \ -e 's|@''HAVE_FSEEKO''@|$(HAVE_FSEEKO)|g' \ -e 's|@''HAVE_FTELLO''@|$(HAVE_FTELLO)|g' \ -e 's|@''HAVE_PCLOSE''@|$(HAVE_PCLOSE)|g' \ -e 's|@''HAVE_POPEN''@|$(HAVE_POPEN)|g' \ -e 's|@''HAVE_RENAMEAT''@|$(HAVE_RENAMEAT)|g' \ -e 's|@''HAVE_VASPRINTF''@|$(HAVE_VASPRINTF)|g' \ -e 's|@''HAVE_VDPRINTF''@|$(HAVE_VDPRINTF)|g' \ -e 's|@''REPLACE_DPRINTF''@|$(REPLACE_DPRINTF)|g' \ -e 's|@''REPLACE_FCLOSE''@|$(REPLACE_FCLOSE)|g' \ -e 's|@''REPLACE_FDOPEN''@|$(REPLACE_FDOPEN)|g' \ -e 's|@''REPLACE_FFLUSH''@|$(REPLACE_FFLUSH)|g' \ -e 's|@''REPLACE_FOPEN''@|$(REPLACE_FOPEN)|g' \ -e 's|@''REPLACE_FPRINTF''@|$(REPLACE_FPRINTF)|g' \ -e 's|@''REPLACE_FPURGE''@|$(REPLACE_FPURGE)|g' \ -e 's|@''REPLACE_FREOPEN''@|$(REPLACE_FREOPEN)|g' \ -e 's|@''REPLACE_FSEEK''@|$(REPLACE_FSEEK)|g' \ -e 's|@''REPLACE_FSEEKO''@|$(REPLACE_FSEEKO)|g' \ -e 's|@''REPLACE_FTELL''@|$(REPLACE_FTELL)|g' \ -e 's|@''REPLACE_FTELLO''@|$(REPLACE_FTELLO)|g' \ -e 's|@''REPLACE_GETDELIM''@|$(REPLACE_GETDELIM)|g' \ -e 's|@''REPLACE_GETLINE''@|$(REPLACE_GETLINE)|g' \ -e 's|@''REPLACE_OBSTACK_PRINTF''@|$(REPLACE_OBSTACK_PRINTF)|g' \ -e 's|@''REPLACE_PERROR''@|$(REPLACE_PERROR)|g' \ -e 's|@''REPLACE_POPEN''@|$(REPLACE_POPEN)|g' \ -e 's|@''REPLACE_PRINTF''@|$(REPLACE_PRINTF)|g' \ -e 's|@''REPLACE_REMOVE''@|$(REPLACE_REMOVE)|g' \ -e 's|@''REPLACE_RENAME''@|$(REPLACE_RENAME)|g' \ -e 's|@''REPLACE_RENAMEAT''@|$(REPLACE_RENAMEAT)|g' \ -e 's|@''REPLACE_SNPRINTF''@|$(REPLACE_SNPRINTF)|g' \ -e 's|@''REPLACE_SPRINTF''@|$(REPLACE_SPRINTF)|g' \ -e 's|@''REPLACE_STDIO_READ_FUNCS''@|$(REPLACE_STDIO_READ_FUNCS)|g' \ -e 's|@''REPLACE_STDIO_WRITE_FUNCS''@|$(REPLACE_STDIO_WRITE_FUNCS)|g' \ -e 's|@''REPLACE_TMPFILE''@|$(REPLACE_TMPFILE)|g' \ -e 's|@''REPLACE_VASPRINTF''@|$(REPLACE_VASPRINTF)|g' \ -e 's|@''REPLACE_VDPRINTF''@|$(REPLACE_VDPRINTF)|g' \ -e 's|@''REPLACE_VFPRINTF''@|$(REPLACE_VFPRINTF)|g' \ -e 's|@''REPLACE_VPRINTF''@|$(REPLACE_VPRINTF)|g' \ -e 's|@''REPLACE_VSNPRINTF''@|$(REPLACE_VSNPRINTF)|g' \ -e 's|@''REPLACE_VSPRINTF''@|$(REPLACE_VSPRINTF)|g' \ -e 's|@''ASM_SYMBOL_PREFIX''@|$(ASM_SYMBOL_PREFIX)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. stdlib.h: stdlib.in.h $(top_builddir)/config.status $(CXXDEFS_H) \ $(_NORETURN_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STDLIB_H''@|$(NEXT_STDLIB_H)|g' \ -e 's/@''GNULIB__EXIT''@/$(GNULIB__EXIT)/g' \ -e 's/@''GNULIB_ATOLL''@/$(GNULIB_ATOLL)/g' \ -e 's/@''GNULIB_CALLOC_POSIX''@/$(GNULIB_CALLOC_POSIX)/g' \ -e 's/@''GNULIB_CANONICALIZE_FILE_NAME''@/$(GNULIB_CANONICALIZE_FILE_NAME)/g' \ -e 's/@''GNULIB_GETLOADAVG''@/$(GNULIB_GETLOADAVG)/g' \ -e 's/@''GNULIB_GETSUBOPT''@/$(GNULIB_GETSUBOPT)/g' \ -e 's/@''GNULIB_GRANTPT''@/$(GNULIB_GRANTPT)/g' \ -e 's/@''GNULIB_MALLOC_POSIX''@/$(GNULIB_MALLOC_POSIX)/g' \ -e 's/@''GNULIB_MBTOWC''@/$(GNULIB_MBTOWC)/g' \ -e 's/@''GNULIB_MKDTEMP''@/$(GNULIB_MKDTEMP)/g' \ -e 's/@''GNULIB_MKOSTEMP''@/$(GNULIB_MKOSTEMP)/g' \ -e 's/@''GNULIB_MKOSTEMPS''@/$(GNULIB_MKOSTEMPS)/g' \ -e 's/@''GNULIB_MKSTEMP''@/$(GNULIB_MKSTEMP)/g' \ -e 's/@''GNULIB_MKSTEMPS''@/$(GNULIB_MKSTEMPS)/g' \ -e 's/@''GNULIB_POSIX_OPENPT''@/$(GNULIB_POSIX_OPENPT)/g' \ -e 's/@''GNULIB_PTSNAME''@/$(GNULIB_PTSNAME)/g' \ -e 's/@''GNULIB_PTSNAME_R''@/$(GNULIB_PTSNAME_R)/g' \ -e 's/@''GNULIB_PUTENV''@/$(GNULIB_PUTENV)/g' \ -e 's/@''GNULIB_QSORT_R''@/$(GNULIB_QSORT_R)/g' \ -e 's/@''GNULIB_RANDOM''@/$(GNULIB_RANDOM)/g' \ -e 's/@''GNULIB_RANDOM_R''@/$(GNULIB_RANDOM_R)/g' \ -e 's/@''GNULIB_REALLOC_POSIX''@/$(GNULIB_REALLOC_POSIX)/g' \ -e 's/@''GNULIB_REALPATH''@/$(GNULIB_REALPATH)/g' \ -e 's/@''GNULIB_RPMATCH''@/$(GNULIB_RPMATCH)/g' \ -e 's/@''GNULIB_SECURE_GETENV''@/$(GNULIB_SECURE_GETENV)/g' \ -e 's/@''GNULIB_SETENV''@/$(GNULIB_SETENV)/g' \ -e 's/@''GNULIB_STRTOD''@/$(GNULIB_STRTOD)/g' \ -e 's/@''GNULIB_STRTOLL''@/$(GNULIB_STRTOLL)/g' \ -e 's/@''GNULIB_STRTOULL''@/$(GNULIB_STRTOULL)/g' \ -e 's/@''GNULIB_SYSTEM_POSIX''@/$(GNULIB_SYSTEM_POSIX)/g' \ -e 's/@''GNULIB_UNLOCKPT''@/$(GNULIB_UNLOCKPT)/g' \ -e 's/@''GNULIB_UNSETENV''@/$(GNULIB_UNSETENV)/g' \ -e 's/@''GNULIB_WCTOMB''@/$(GNULIB_WCTOMB)/g' \ < $(srcdir)/stdlib.in.h | \ sed -e 's|@''HAVE__EXIT''@|$(HAVE__EXIT)|g' \ -e 's|@''HAVE_ATOLL''@|$(HAVE_ATOLL)|g' \ -e 's|@''HAVE_CANONICALIZE_FILE_NAME''@|$(HAVE_CANONICALIZE_FILE_NAME)|g' \ -e 's|@''HAVE_DECL_GETLOADAVG''@|$(HAVE_DECL_GETLOADAVG)|g' \ -e 's|@''HAVE_GETSUBOPT''@|$(HAVE_GETSUBOPT)|g' \ -e 's|@''HAVE_GRANTPT''@|$(HAVE_GRANTPT)|g' \ -e 's|@''HAVE_MKDTEMP''@|$(HAVE_MKDTEMP)|g' \ -e 's|@''HAVE_MKOSTEMP''@|$(HAVE_MKOSTEMP)|g' \ -e 's|@''HAVE_MKOSTEMPS''@|$(HAVE_MKOSTEMPS)|g' \ -e 's|@''HAVE_MKSTEMP''@|$(HAVE_MKSTEMP)|g' \ -e 's|@''HAVE_MKSTEMPS''@|$(HAVE_MKSTEMPS)|g' \ -e 's|@''HAVE_POSIX_OPENPT''@|$(HAVE_POSIX_OPENPT)|g' \ -e 's|@''HAVE_PTSNAME''@|$(HAVE_PTSNAME)|g' \ -e 's|@''HAVE_PTSNAME_R''@|$(HAVE_PTSNAME_R)|g' \ -e 's|@''HAVE_QSORT_R''@|$(HAVE_QSORT_R)|g' \ -e 's|@''HAVE_RANDOM''@|$(HAVE_RANDOM)|g' \ -e 's|@''HAVE_RANDOM_H''@|$(HAVE_RANDOM_H)|g' \ -e 's|@''HAVE_RANDOM_R''@|$(HAVE_RANDOM_R)|g' \ -e 's|@''HAVE_REALPATH''@|$(HAVE_REALPATH)|g' \ -e 's|@''HAVE_RPMATCH''@|$(HAVE_RPMATCH)|g' \ -e 's|@''HAVE_SECURE_GETENV''@|$(HAVE_SECURE_GETENV)|g' \ -e 's|@''HAVE_DECL_SETENV''@|$(HAVE_DECL_SETENV)|g' \ -e 's|@''HAVE_STRTOD''@|$(HAVE_STRTOD)|g' \ -e 's|@''HAVE_STRTOLL''@|$(HAVE_STRTOLL)|g' \ -e 's|@''HAVE_STRTOULL''@|$(HAVE_STRTOULL)|g' \ -e 's|@''HAVE_STRUCT_RANDOM_DATA''@|$(HAVE_STRUCT_RANDOM_DATA)|g' \ -e 's|@''HAVE_SYS_LOADAVG_H''@|$(HAVE_SYS_LOADAVG_H)|g' \ -e 's|@''HAVE_UNLOCKPT''@|$(HAVE_UNLOCKPT)|g' \ -e 's|@''HAVE_DECL_UNSETENV''@|$(HAVE_DECL_UNSETENV)|g' \ -e 's|@''REPLACE_CALLOC''@|$(REPLACE_CALLOC)|g' \ -e 's|@''REPLACE_CANONICALIZE_FILE_NAME''@|$(REPLACE_CANONICALIZE_FILE_NAME)|g' \ -e 's|@''REPLACE_MALLOC''@|$(REPLACE_MALLOC)|g' \ -e 's|@''REPLACE_MBTOWC''@|$(REPLACE_MBTOWC)|g' \ -e 's|@''REPLACE_MKSTEMP''@|$(REPLACE_MKSTEMP)|g' \ -e 's|@''REPLACE_PTSNAME''@|$(REPLACE_PTSNAME)|g' \ -e 's|@''REPLACE_PTSNAME_R''@|$(REPLACE_PTSNAME_R)|g' \ -e 's|@''REPLACE_PUTENV''@|$(REPLACE_PUTENV)|g' \ -e 's|@''REPLACE_QSORT_R''@|$(REPLACE_QSORT_R)|g' \ -e 's|@''REPLACE_RANDOM_R''@|$(REPLACE_RANDOM_R)|g' \ -e 's|@''REPLACE_REALLOC''@|$(REPLACE_REALLOC)|g' \ -e 's|@''REPLACE_REALPATH''@|$(REPLACE_REALPATH)|g' \ -e 's|@''REPLACE_SETENV''@|$(REPLACE_SETENV)|g' \ -e 's|@''REPLACE_STRTOD''@|$(REPLACE_STRTOD)|g' \ -e 's|@''REPLACE_UNSETENV''@|$(REPLACE_UNSETENV)|g' \ -e 's|@''REPLACE_WCTOMB''@|$(REPLACE_WCTOMB)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _Noreturn/r $(_NORETURN_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. string.h: string.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STRING_H''@|$(NEXT_STRING_H)|g' \ -e 's/@''GNULIB_FFSL''@/$(GNULIB_FFSL)/g' \ -e 's/@''GNULIB_FFSLL''@/$(GNULIB_FFSLL)/g' \ -e 's/@''GNULIB_MBSLEN''@/$(GNULIB_MBSLEN)/g' \ -e 's/@''GNULIB_MBSNLEN''@/$(GNULIB_MBSNLEN)/g' \ -e 's/@''GNULIB_MBSCHR''@/$(GNULIB_MBSCHR)/g' \ -e 's/@''GNULIB_MBSRCHR''@/$(GNULIB_MBSRCHR)/g' \ -e 's/@''GNULIB_MBSSTR''@/$(GNULIB_MBSSTR)/g' \ -e 's/@''GNULIB_MBSCASECMP''@/$(GNULIB_MBSCASECMP)/g' \ -e 's/@''GNULIB_MBSNCASECMP''@/$(GNULIB_MBSNCASECMP)/g' \ -e 's/@''GNULIB_MBSPCASECMP''@/$(GNULIB_MBSPCASECMP)/g' \ -e 's/@''GNULIB_MBSCASESTR''@/$(GNULIB_MBSCASESTR)/g' \ -e 's/@''GNULIB_MBSCSPN''@/$(GNULIB_MBSCSPN)/g' \ -e 's/@''GNULIB_MBSPBRK''@/$(GNULIB_MBSPBRK)/g' \ -e 's/@''GNULIB_MBSSPN''@/$(GNULIB_MBSSPN)/g' \ -e 's/@''GNULIB_MBSSEP''@/$(GNULIB_MBSSEP)/g' \ -e 's/@''GNULIB_MBSTOK_R''@/$(GNULIB_MBSTOK_R)/g' \ -e 's/@''GNULIB_MEMCHR''@/$(GNULIB_MEMCHR)/g' \ -e 's/@''GNULIB_MEMMEM''@/$(GNULIB_MEMMEM)/g' \ -e 's/@''GNULIB_MEMPCPY''@/$(GNULIB_MEMPCPY)/g' \ -e 's/@''GNULIB_MEMRCHR''@/$(GNULIB_MEMRCHR)/g' \ -e 's/@''GNULIB_RAWMEMCHR''@/$(GNULIB_RAWMEMCHR)/g' \ -e 's/@''GNULIB_STPCPY''@/$(GNULIB_STPCPY)/g' \ -e 's/@''GNULIB_STPNCPY''@/$(GNULIB_STPNCPY)/g' \ -e 's/@''GNULIB_STRCHRNUL''@/$(GNULIB_STRCHRNUL)/g' \ -e 's/@''GNULIB_STRDUP''@/$(GNULIB_STRDUP)/g' \ -e 's/@''GNULIB_STRNCAT''@/$(GNULIB_STRNCAT)/g' \ -e 's/@''GNULIB_STRNDUP''@/$(GNULIB_STRNDUP)/g' \ -e 's/@''GNULIB_STRNLEN''@/$(GNULIB_STRNLEN)/g' \ -e 's/@''GNULIB_STRPBRK''@/$(GNULIB_STRPBRK)/g' \ -e 's/@''GNULIB_STRSEP''@/$(GNULIB_STRSEP)/g' \ -e 's/@''GNULIB_STRSTR''@/$(GNULIB_STRSTR)/g' \ -e 's/@''GNULIB_STRCASESTR''@/$(GNULIB_STRCASESTR)/g' \ -e 's/@''GNULIB_STRTOK_R''@/$(GNULIB_STRTOK_R)/g' \ -e 's/@''GNULIB_STRERROR''@/$(GNULIB_STRERROR)/g' \ -e 's/@''GNULIB_STRERROR_R''@/$(GNULIB_STRERROR_R)/g' \ -e 's/@''GNULIB_STRSIGNAL''@/$(GNULIB_STRSIGNAL)/g' \ -e 's/@''GNULIB_STRVERSCMP''@/$(GNULIB_STRVERSCMP)/g' \ < $(srcdir)/string.in.h | \ sed -e 's|@''HAVE_FFSL''@|$(HAVE_FFSL)|g' \ -e 's|@''HAVE_FFSLL''@|$(HAVE_FFSLL)|g' \ -e 's|@''HAVE_MBSLEN''@|$(HAVE_MBSLEN)|g' \ -e 's|@''HAVE_MEMCHR''@|$(HAVE_MEMCHR)|g' \ -e 's|@''HAVE_DECL_MEMMEM''@|$(HAVE_DECL_MEMMEM)|g' \ -e 's|@''HAVE_MEMPCPY''@|$(HAVE_MEMPCPY)|g' \ -e 's|@''HAVE_DECL_MEMRCHR''@|$(HAVE_DECL_MEMRCHR)|g' \ -e 's|@''HAVE_RAWMEMCHR''@|$(HAVE_RAWMEMCHR)|g' \ -e 's|@''HAVE_STPCPY''@|$(HAVE_STPCPY)|g' \ -e 's|@''HAVE_STPNCPY''@|$(HAVE_STPNCPY)|g' \ -e 's|@''HAVE_STRCHRNUL''@|$(HAVE_STRCHRNUL)|g' \ -e 's|@''HAVE_DECL_STRDUP''@|$(HAVE_DECL_STRDUP)|g' \ -e 's|@''HAVE_DECL_STRNDUP''@|$(HAVE_DECL_STRNDUP)|g' \ -e 's|@''HAVE_DECL_STRNLEN''@|$(HAVE_DECL_STRNLEN)|g' \ -e 's|@''HAVE_STRPBRK''@|$(HAVE_STRPBRK)|g' \ -e 's|@''HAVE_STRSEP''@|$(HAVE_STRSEP)|g' \ -e 's|@''HAVE_STRCASESTR''@|$(HAVE_STRCASESTR)|g' \ -e 's|@''HAVE_DECL_STRTOK_R''@|$(HAVE_DECL_STRTOK_R)|g' \ -e 's|@''HAVE_DECL_STRERROR_R''@|$(HAVE_DECL_STRERROR_R)|g' \ -e 's|@''HAVE_DECL_STRSIGNAL''@|$(HAVE_DECL_STRSIGNAL)|g' \ -e 's|@''HAVE_STRVERSCMP''@|$(HAVE_STRVERSCMP)|g' \ -e 's|@''REPLACE_STPNCPY''@|$(REPLACE_STPNCPY)|g' \ -e 's|@''REPLACE_MEMCHR''@|$(REPLACE_MEMCHR)|g' \ -e 's|@''REPLACE_MEMMEM''@|$(REPLACE_MEMMEM)|g' \ -e 's|@''REPLACE_STRCASESTR''@|$(REPLACE_STRCASESTR)|g' \ -e 's|@''REPLACE_STRCHRNUL''@|$(REPLACE_STRCHRNUL)|g' \ -e 's|@''REPLACE_STRDUP''@|$(REPLACE_STRDUP)|g' \ -e 's|@''REPLACE_STRSTR''@|$(REPLACE_STRSTR)|g' \ -e 's|@''REPLACE_STRERROR''@|$(REPLACE_STRERROR)|g' \ -e 's|@''REPLACE_STRERROR_R''@|$(REPLACE_STRERROR_R)|g' \ -e 's|@''REPLACE_STRNCAT''@|$(REPLACE_STRNCAT)|g' \ -e 's|@''REPLACE_STRNDUP''@|$(REPLACE_STRNDUP)|g' \ -e 's|@''REPLACE_STRNLEN''@|$(REPLACE_STRNLEN)|g' \ -e 's|@''REPLACE_STRSIGNAL''@|$(REPLACE_STRSIGNAL)|g' \ -e 's|@''REPLACE_STRTOK_R''@|$(REPLACE_STRTOK_R)|g' \ -e 's|@''UNDEFINE_STRTOK_R''@|$(UNDEFINE_STRTOK_R)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ < $(srcdir)/string.in.h; \ } > $@-t && \ mv $@-t $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. strings.h: strings.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(ARG_NONNULL_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''HAVE_STRINGS_H''@|$(HAVE_STRINGS_H)|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STRINGS_H''@|$(NEXT_STRINGS_H)|g' \ -e 's|@''GNULIB_FFS''@|$(GNULIB_FFS)|g' \ -e 's|@''HAVE_FFS''@|$(HAVE_FFS)|g' \ -e 's|@''HAVE_STRCASECMP''@|$(HAVE_STRCASECMP)|g' \ -e 's|@''HAVE_DECL_STRNCASECMP''@|$(HAVE_DECL_STRNCASECMP)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/strings.in.h; \ } > $@-t && \ mv $@-t $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. sys/types.h: sys_types.in.h $(top_builddir)/config.status $(AM_V_at)$(MKDIR_P) sys $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_SYS_TYPES_H''@|$(NEXT_SYS_TYPES_H)|g' \ -e 's|@''WINDOWS_64_BIT_OFF_T''@|$(WINDOWS_64_BIT_OFF_T)|g' \ < $(srcdir)/sys_types.in.h; \ } > $@-t && \ mv $@-t $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. @GL_GENERATE_SYSEXITS_H_TRUE@sysexits.h: sysexits.in.h $(top_builddir)/config.status @GL_GENERATE_SYSEXITS_H_TRUE@ $(AM_V_GEN)rm -f $@-t $@ && \ @GL_GENERATE_SYSEXITS_H_TRUE@ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ @GL_GENERATE_SYSEXITS_H_TRUE@ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ @GL_GENERATE_SYSEXITS_H_TRUE@ -e 's|@''HAVE_SYSEXITS_H''@|$(HAVE_SYSEXITS_H)|g' \ @GL_GENERATE_SYSEXITS_H_TRUE@ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ @GL_GENERATE_SYSEXITS_H_TRUE@ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ @GL_GENERATE_SYSEXITS_H_TRUE@ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ @GL_GENERATE_SYSEXITS_H_TRUE@ -e 's|@''NEXT_SYSEXITS_H''@|$(NEXT_SYSEXITS_H)|g' \ @GL_GENERATE_SYSEXITS_H_TRUE@ < $(srcdir)/sysexits.in.h; \ @GL_GENERATE_SYSEXITS_H_TRUE@ } > $@-t && \ @GL_GENERATE_SYSEXITS_H_TRUE@ mv -f $@-t $@ @GL_GENERATE_SYSEXITS_H_FALSE@sysexits.h: $(top_builddir)/config.status @GL_GENERATE_SYSEXITS_H_FALSE@ rm -f $@ # We need the following in order to create an empty placeholder for # when the system doesn't have one. unistd.h: unistd.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''HAVE_UNISTD_H''@|$(HAVE_UNISTD_H)|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_UNISTD_H''@|$(NEXT_UNISTD_H)|g' \ -e 's|@''WINDOWS_64_BIT_OFF_T''@|$(WINDOWS_64_BIT_OFF_T)|g' \ -e 's/@''GNULIB_CHDIR''@/$(GNULIB_CHDIR)/g' \ -e 's/@''GNULIB_CHOWN''@/$(GNULIB_CHOWN)/g' \ -e 's/@''GNULIB_CLOSE''@/$(GNULIB_CLOSE)/g' \ -e 's/@''GNULIB_DUP''@/$(GNULIB_DUP)/g' \ -e 's/@''GNULIB_DUP2''@/$(GNULIB_DUP2)/g' \ -e 's/@''GNULIB_DUP3''@/$(GNULIB_DUP3)/g' \ -e 's/@''GNULIB_ENVIRON''@/$(GNULIB_ENVIRON)/g' \ -e 's/@''GNULIB_EUIDACCESS''@/$(GNULIB_EUIDACCESS)/g' \ -e 's/@''GNULIB_FACCESSAT''@/$(GNULIB_FACCESSAT)/g' \ -e 's/@''GNULIB_FCHDIR''@/$(GNULIB_FCHDIR)/g' \ -e 's/@''GNULIB_FCHOWNAT''@/$(GNULIB_FCHOWNAT)/g' \ -e 's/@''GNULIB_FDATASYNC''@/$(GNULIB_FDATASYNC)/g' \ -e 's/@''GNULIB_FSYNC''@/$(GNULIB_FSYNC)/g' \ -e 's/@''GNULIB_FTRUNCATE''@/$(GNULIB_FTRUNCATE)/g' \ -e 's/@''GNULIB_GETCWD''@/$(GNULIB_GETCWD)/g' \ -e 's/@''GNULIB_GETDOMAINNAME''@/$(GNULIB_GETDOMAINNAME)/g' \ -e 's/@''GNULIB_GETDTABLESIZE''@/$(GNULIB_GETDTABLESIZE)/g' \ -e 's/@''GNULIB_GETGROUPS''@/$(GNULIB_GETGROUPS)/g' \ -e 's/@''GNULIB_GETHOSTNAME''@/$(GNULIB_GETHOSTNAME)/g' \ -e 's/@''GNULIB_GETLOGIN''@/$(GNULIB_GETLOGIN)/g' \ -e 's/@''GNULIB_GETLOGIN_R''@/$(GNULIB_GETLOGIN_R)/g' \ -e 's/@''GNULIB_GETPAGESIZE''@/$(GNULIB_GETPAGESIZE)/g' \ -e 's/@''GNULIB_GETUSERSHELL''@/$(GNULIB_GETUSERSHELL)/g' \ -e 's/@''GNULIB_GROUP_MEMBER''@/$(GNULIB_GROUP_MEMBER)/g' \ -e 's/@''GNULIB_ISATTY''@/$(GNULIB_ISATTY)/g' \ -e 's/@''GNULIB_LCHOWN''@/$(GNULIB_LCHOWN)/g' \ -e 's/@''GNULIB_LINK''@/$(GNULIB_LINK)/g' \ -e 's/@''GNULIB_LINKAT''@/$(GNULIB_LINKAT)/g' \ -e 's/@''GNULIB_LSEEK''@/$(GNULIB_LSEEK)/g' \ -e 's/@''GNULIB_PIPE''@/$(GNULIB_PIPE)/g' \ -e 's/@''GNULIB_PIPE2''@/$(GNULIB_PIPE2)/g' \ -e 's/@''GNULIB_PREAD''@/$(GNULIB_PREAD)/g' \ -e 's/@''GNULIB_PWRITE''@/$(GNULIB_PWRITE)/g' \ -e 's/@''GNULIB_READ''@/$(GNULIB_READ)/g' \ -e 's/@''GNULIB_READLINK''@/$(GNULIB_READLINK)/g' \ -e 's/@''GNULIB_READLINKAT''@/$(GNULIB_READLINKAT)/g' \ -e 's/@''GNULIB_RMDIR''@/$(GNULIB_RMDIR)/g' \ -e 's/@''GNULIB_SETHOSTNAME''@/$(GNULIB_SETHOSTNAME)/g' \ -e 's/@''GNULIB_SLEEP''@/$(GNULIB_SLEEP)/g' \ -e 's/@''GNULIB_SYMLINK''@/$(GNULIB_SYMLINK)/g' \ -e 's/@''GNULIB_SYMLINKAT''@/$(GNULIB_SYMLINKAT)/g' \ -e 's/@''GNULIB_TTYNAME_R''@/$(GNULIB_TTYNAME_R)/g' \ -e 's/@''GNULIB_UNISTD_H_GETOPT''@/0$(GNULIB_GL_UNISTD_H_GETOPT)/g' \ -e 's/@''GNULIB_UNISTD_H_NONBLOCKING''@/$(GNULIB_UNISTD_H_NONBLOCKING)/g' \ -e 's/@''GNULIB_UNISTD_H_SIGPIPE''@/$(GNULIB_UNISTD_H_SIGPIPE)/g' \ -e 's/@''GNULIB_UNLINK''@/$(GNULIB_UNLINK)/g' \ -e 's/@''GNULIB_UNLINKAT''@/$(GNULIB_UNLINKAT)/g' \ -e 's/@''GNULIB_USLEEP''@/$(GNULIB_USLEEP)/g' \ -e 's/@''GNULIB_WRITE''@/$(GNULIB_WRITE)/g' \ < $(srcdir)/unistd.in.h | \ sed -e 's|@''HAVE_CHOWN''@|$(HAVE_CHOWN)|g' \ -e 's|@''HAVE_DUP2''@|$(HAVE_DUP2)|g' \ -e 's|@''HAVE_DUP3''@|$(HAVE_DUP3)|g' \ -e 's|@''HAVE_EUIDACCESS''@|$(HAVE_EUIDACCESS)|g' \ -e 's|@''HAVE_FACCESSAT''@|$(HAVE_FACCESSAT)|g' \ -e 's|@''HAVE_FCHDIR''@|$(HAVE_FCHDIR)|g' \ -e 's|@''HAVE_FCHOWNAT''@|$(HAVE_FCHOWNAT)|g' \ -e 's|@''HAVE_FDATASYNC''@|$(HAVE_FDATASYNC)|g' \ -e 's|@''HAVE_FSYNC''@|$(HAVE_FSYNC)|g' \ -e 's|@''HAVE_FTRUNCATE''@|$(HAVE_FTRUNCATE)|g' \ -e 's|@''HAVE_GETDTABLESIZE''@|$(HAVE_GETDTABLESIZE)|g' \ -e 's|@''HAVE_GETGROUPS''@|$(HAVE_GETGROUPS)|g' \ -e 's|@''HAVE_GETHOSTNAME''@|$(HAVE_GETHOSTNAME)|g' \ -e 's|@''HAVE_GETLOGIN''@|$(HAVE_GETLOGIN)|g' \ -e 's|@''HAVE_GETPAGESIZE''@|$(HAVE_GETPAGESIZE)|g' \ -e 's|@''HAVE_GROUP_MEMBER''@|$(HAVE_GROUP_MEMBER)|g' \ -e 's|@''HAVE_LCHOWN''@|$(HAVE_LCHOWN)|g' \ -e 's|@''HAVE_LINK''@|$(HAVE_LINK)|g' \ -e 's|@''HAVE_LINKAT''@|$(HAVE_LINKAT)|g' \ -e 's|@''HAVE_PIPE''@|$(HAVE_PIPE)|g' \ -e 's|@''HAVE_PIPE2''@|$(HAVE_PIPE2)|g' \ -e 's|@''HAVE_PREAD''@|$(HAVE_PREAD)|g' \ -e 's|@''HAVE_PWRITE''@|$(HAVE_PWRITE)|g' \ -e 's|@''HAVE_READLINK''@|$(HAVE_READLINK)|g' \ -e 's|@''HAVE_READLINKAT''@|$(HAVE_READLINKAT)|g' \ -e 's|@''HAVE_SETHOSTNAME''@|$(HAVE_SETHOSTNAME)|g' \ -e 's|@''HAVE_SLEEP''@|$(HAVE_SLEEP)|g' \ -e 's|@''HAVE_SYMLINK''@|$(HAVE_SYMLINK)|g' \ -e 's|@''HAVE_SYMLINKAT''@|$(HAVE_SYMLINKAT)|g' \ -e 's|@''HAVE_UNLINKAT''@|$(HAVE_UNLINKAT)|g' \ -e 's|@''HAVE_USLEEP''@|$(HAVE_USLEEP)|g' \ -e 's|@''HAVE_DECL_ENVIRON''@|$(HAVE_DECL_ENVIRON)|g' \ -e 's|@''HAVE_DECL_FCHDIR''@|$(HAVE_DECL_FCHDIR)|g' \ -e 's|@''HAVE_DECL_FDATASYNC''@|$(HAVE_DECL_FDATASYNC)|g' \ -e 's|@''HAVE_DECL_GETDOMAINNAME''@|$(HAVE_DECL_GETDOMAINNAME)|g' \ -e 's|@''HAVE_DECL_GETLOGIN_R''@|$(HAVE_DECL_GETLOGIN_R)|g' \ -e 's|@''HAVE_DECL_GETPAGESIZE''@|$(HAVE_DECL_GETPAGESIZE)|g' \ -e 's|@''HAVE_DECL_GETUSERSHELL''@|$(HAVE_DECL_GETUSERSHELL)|g' \ -e 's|@''HAVE_DECL_SETHOSTNAME''@|$(HAVE_DECL_SETHOSTNAME)|g' \ -e 's|@''HAVE_DECL_TTYNAME_R''@|$(HAVE_DECL_TTYNAME_R)|g' \ -e 's|@''HAVE_OS_H''@|$(HAVE_OS_H)|g' \ -e 's|@''HAVE_SYS_PARAM_H''@|$(HAVE_SYS_PARAM_H)|g' \ | \ sed -e 's|@''REPLACE_CHOWN''@|$(REPLACE_CHOWN)|g' \ -e 's|@''REPLACE_CLOSE''@|$(REPLACE_CLOSE)|g' \ -e 's|@''REPLACE_DUP''@|$(REPLACE_DUP)|g' \ -e 's|@''REPLACE_DUP2''@|$(REPLACE_DUP2)|g' \ -e 's|@''REPLACE_FCHOWNAT''@|$(REPLACE_FCHOWNAT)|g' \ -e 's|@''REPLACE_FTRUNCATE''@|$(REPLACE_FTRUNCATE)|g' \ -e 's|@''REPLACE_GETCWD''@|$(REPLACE_GETCWD)|g' \ -e 's|@''REPLACE_GETDOMAINNAME''@|$(REPLACE_GETDOMAINNAME)|g' \ -e 's|@''REPLACE_GETDTABLESIZE''@|$(REPLACE_GETDTABLESIZE)|g' \ -e 's|@''REPLACE_GETLOGIN_R''@|$(REPLACE_GETLOGIN_R)|g' \ -e 's|@''REPLACE_GETGROUPS''@|$(REPLACE_GETGROUPS)|g' \ -e 's|@''REPLACE_GETPAGESIZE''@|$(REPLACE_GETPAGESIZE)|g' \ -e 's|@''REPLACE_ISATTY''@|$(REPLACE_ISATTY)|g' \ -e 's|@''REPLACE_LCHOWN''@|$(REPLACE_LCHOWN)|g' \ -e 's|@''REPLACE_LINK''@|$(REPLACE_LINK)|g' \ -e 's|@''REPLACE_LINKAT''@|$(REPLACE_LINKAT)|g' \ -e 's|@''REPLACE_LSEEK''@|$(REPLACE_LSEEK)|g' \ -e 's|@''REPLACE_PREAD''@|$(REPLACE_PREAD)|g' \ -e 's|@''REPLACE_PWRITE''@|$(REPLACE_PWRITE)|g' \ -e 's|@''REPLACE_READ''@|$(REPLACE_READ)|g' \ -e 's|@''REPLACE_READLINK''@|$(REPLACE_READLINK)|g' \ -e 's|@''REPLACE_READLINKAT''@|$(REPLACE_READLINKAT)|g' \ -e 's|@''REPLACE_RMDIR''@|$(REPLACE_RMDIR)|g' \ -e 's|@''REPLACE_SLEEP''@|$(REPLACE_SLEEP)|g' \ -e 's|@''REPLACE_SYMLINK''@|$(REPLACE_SYMLINK)|g' \ -e 's|@''REPLACE_SYMLINKAT''@|$(REPLACE_SYMLINKAT)|g' \ -e 's|@''REPLACE_TTYNAME_R''@|$(REPLACE_TTYNAME_R)|g' \ -e 's|@''REPLACE_UNLINK''@|$(REPLACE_UNLINK)|g' \ -e 's|@''REPLACE_UNLINKAT''@|$(REPLACE_UNLINKAT)|g' \ -e 's|@''REPLACE_USLEEP''@|$(REPLACE_USLEEP)|g' \ -e 's|@''REPLACE_WRITE''@|$(REPLACE_WRITE)|g' \ -e 's|@''UNISTD_H_HAVE_WINSOCK2_H''@|$(UNISTD_H_HAVE_WINSOCK2_H)|g' \ -e 's|@''UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS''@|$(UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ # We need the following in order to create when the system # version does not work standalone. wchar.h: wchar.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''HAVE_FEATURES_H''@|$(HAVE_FEATURES_H)|g' \ -e 's|@''NEXT_WCHAR_H''@|$(NEXT_WCHAR_H)|g' \ -e 's|@''HAVE_WCHAR_H''@|$(HAVE_WCHAR_H)|g' \ -e 's/@''GNULIB_BTOWC''@/$(GNULIB_BTOWC)/g' \ -e 's/@''GNULIB_WCTOB''@/$(GNULIB_WCTOB)/g' \ -e 's/@''GNULIB_MBSINIT''@/$(GNULIB_MBSINIT)/g' \ -e 's/@''GNULIB_MBRTOWC''@/$(GNULIB_MBRTOWC)/g' \ -e 's/@''GNULIB_MBRLEN''@/$(GNULIB_MBRLEN)/g' \ -e 's/@''GNULIB_MBSRTOWCS''@/$(GNULIB_MBSRTOWCS)/g' \ -e 's/@''GNULIB_MBSNRTOWCS''@/$(GNULIB_MBSNRTOWCS)/g' \ -e 's/@''GNULIB_WCRTOMB''@/$(GNULIB_WCRTOMB)/g' \ -e 's/@''GNULIB_WCSRTOMBS''@/$(GNULIB_WCSRTOMBS)/g' \ -e 's/@''GNULIB_WCSNRTOMBS''@/$(GNULIB_WCSNRTOMBS)/g' \ -e 's/@''GNULIB_WCWIDTH''@/$(GNULIB_WCWIDTH)/g' \ -e 's/@''GNULIB_WMEMCHR''@/$(GNULIB_WMEMCHR)/g' \ -e 's/@''GNULIB_WMEMCMP''@/$(GNULIB_WMEMCMP)/g' \ -e 's/@''GNULIB_WMEMCPY''@/$(GNULIB_WMEMCPY)/g' \ -e 's/@''GNULIB_WMEMMOVE''@/$(GNULIB_WMEMMOVE)/g' \ -e 's/@''GNULIB_WMEMSET''@/$(GNULIB_WMEMSET)/g' \ -e 's/@''GNULIB_WCSLEN''@/$(GNULIB_WCSLEN)/g' \ -e 's/@''GNULIB_WCSNLEN''@/$(GNULIB_WCSNLEN)/g' \ -e 's/@''GNULIB_WCSCPY''@/$(GNULIB_WCSCPY)/g' \ -e 's/@''GNULIB_WCPCPY''@/$(GNULIB_WCPCPY)/g' \ -e 's/@''GNULIB_WCSNCPY''@/$(GNULIB_WCSNCPY)/g' \ -e 's/@''GNULIB_WCPNCPY''@/$(GNULIB_WCPNCPY)/g' \ -e 's/@''GNULIB_WCSCAT''@/$(GNULIB_WCSCAT)/g' \ -e 's/@''GNULIB_WCSNCAT''@/$(GNULIB_WCSNCAT)/g' \ -e 's/@''GNULIB_WCSCMP''@/$(GNULIB_WCSCMP)/g' \ -e 's/@''GNULIB_WCSNCMP''@/$(GNULIB_WCSNCMP)/g' \ -e 's/@''GNULIB_WCSCASECMP''@/$(GNULIB_WCSCASECMP)/g' \ -e 's/@''GNULIB_WCSNCASECMP''@/$(GNULIB_WCSNCASECMP)/g' \ -e 's/@''GNULIB_WCSCOLL''@/$(GNULIB_WCSCOLL)/g' \ -e 's/@''GNULIB_WCSXFRM''@/$(GNULIB_WCSXFRM)/g' \ -e 's/@''GNULIB_WCSDUP''@/$(GNULIB_WCSDUP)/g' \ -e 's/@''GNULIB_WCSCHR''@/$(GNULIB_WCSCHR)/g' \ -e 's/@''GNULIB_WCSRCHR''@/$(GNULIB_WCSRCHR)/g' \ -e 's/@''GNULIB_WCSCSPN''@/$(GNULIB_WCSCSPN)/g' \ -e 's/@''GNULIB_WCSSPN''@/$(GNULIB_WCSSPN)/g' \ -e 's/@''GNULIB_WCSPBRK''@/$(GNULIB_WCSPBRK)/g' \ -e 's/@''GNULIB_WCSSTR''@/$(GNULIB_WCSSTR)/g' \ -e 's/@''GNULIB_WCSTOK''@/$(GNULIB_WCSTOK)/g' \ -e 's/@''GNULIB_WCSWIDTH''@/$(GNULIB_WCSWIDTH)/g' \ < $(srcdir)/wchar.in.h | \ sed -e 's|@''HAVE_WINT_T''@|$(HAVE_WINT_T)|g' \ -e 's|@''HAVE_BTOWC''@|$(HAVE_BTOWC)|g' \ -e 's|@''HAVE_MBSINIT''@|$(HAVE_MBSINIT)|g' \ -e 's|@''HAVE_MBRTOWC''@|$(HAVE_MBRTOWC)|g' \ -e 's|@''HAVE_MBRLEN''@|$(HAVE_MBRLEN)|g' \ -e 's|@''HAVE_MBSRTOWCS''@|$(HAVE_MBSRTOWCS)|g' \ -e 's|@''HAVE_MBSNRTOWCS''@|$(HAVE_MBSNRTOWCS)|g' \ -e 's|@''HAVE_WCRTOMB''@|$(HAVE_WCRTOMB)|g' \ -e 's|@''HAVE_WCSRTOMBS''@|$(HAVE_WCSRTOMBS)|g' \ -e 's|@''HAVE_WCSNRTOMBS''@|$(HAVE_WCSNRTOMBS)|g' \ -e 's|@''HAVE_WMEMCHR''@|$(HAVE_WMEMCHR)|g' \ -e 's|@''HAVE_WMEMCMP''@|$(HAVE_WMEMCMP)|g' \ -e 's|@''HAVE_WMEMCPY''@|$(HAVE_WMEMCPY)|g' \ -e 's|@''HAVE_WMEMMOVE''@|$(HAVE_WMEMMOVE)|g' \ -e 's|@''HAVE_WMEMSET''@|$(HAVE_WMEMSET)|g' \ -e 's|@''HAVE_WCSLEN''@|$(HAVE_WCSLEN)|g' \ -e 's|@''HAVE_WCSNLEN''@|$(HAVE_WCSNLEN)|g' \ -e 's|@''HAVE_WCSCPY''@|$(HAVE_WCSCPY)|g' \ -e 's|@''HAVE_WCPCPY''@|$(HAVE_WCPCPY)|g' \ -e 's|@''HAVE_WCSNCPY''@|$(HAVE_WCSNCPY)|g' \ -e 's|@''HAVE_WCPNCPY''@|$(HAVE_WCPNCPY)|g' \ -e 's|@''HAVE_WCSCAT''@|$(HAVE_WCSCAT)|g' \ -e 's|@''HAVE_WCSNCAT''@|$(HAVE_WCSNCAT)|g' \ -e 's|@''HAVE_WCSCMP''@|$(HAVE_WCSCMP)|g' \ -e 's|@''HAVE_WCSNCMP''@|$(HAVE_WCSNCMP)|g' \ -e 's|@''HAVE_WCSCASECMP''@|$(HAVE_WCSCASECMP)|g' \ -e 's|@''HAVE_WCSNCASECMP''@|$(HAVE_WCSNCASECMP)|g' \ -e 's|@''HAVE_WCSCOLL''@|$(HAVE_WCSCOLL)|g' \ -e 's|@''HAVE_WCSXFRM''@|$(HAVE_WCSXFRM)|g' \ -e 's|@''HAVE_WCSDUP''@|$(HAVE_WCSDUP)|g' \ -e 's|@''HAVE_WCSCHR''@|$(HAVE_WCSCHR)|g' \ -e 's|@''HAVE_WCSRCHR''@|$(HAVE_WCSRCHR)|g' \ -e 's|@''HAVE_WCSCSPN''@|$(HAVE_WCSCSPN)|g' \ -e 's|@''HAVE_WCSSPN''@|$(HAVE_WCSSPN)|g' \ -e 's|@''HAVE_WCSPBRK''@|$(HAVE_WCSPBRK)|g' \ -e 's|@''HAVE_WCSSTR''@|$(HAVE_WCSSTR)|g' \ -e 's|@''HAVE_WCSTOK''@|$(HAVE_WCSTOK)|g' \ -e 's|@''HAVE_WCSWIDTH''@|$(HAVE_WCSWIDTH)|g' \ -e 's|@''HAVE_DECL_WCTOB''@|$(HAVE_DECL_WCTOB)|g' \ -e 's|@''HAVE_DECL_WCWIDTH''@|$(HAVE_DECL_WCWIDTH)|g' \ | \ sed -e 's|@''REPLACE_MBSTATE_T''@|$(REPLACE_MBSTATE_T)|g' \ -e 's|@''REPLACE_BTOWC''@|$(REPLACE_BTOWC)|g' \ -e 's|@''REPLACE_WCTOB''@|$(REPLACE_WCTOB)|g' \ -e 's|@''REPLACE_MBSINIT''@|$(REPLACE_MBSINIT)|g' \ -e 's|@''REPLACE_MBRTOWC''@|$(REPLACE_MBRTOWC)|g' \ -e 's|@''REPLACE_MBRLEN''@|$(REPLACE_MBRLEN)|g' \ -e 's|@''REPLACE_MBSRTOWCS''@|$(REPLACE_MBSRTOWCS)|g' \ -e 's|@''REPLACE_MBSNRTOWCS''@|$(REPLACE_MBSNRTOWCS)|g' \ -e 's|@''REPLACE_WCRTOMB''@|$(REPLACE_WCRTOMB)|g' \ -e 's|@''REPLACE_WCSRTOMBS''@|$(REPLACE_WCSRTOMBS)|g' \ -e 's|@''REPLACE_WCSNRTOMBS''@|$(REPLACE_WCSNRTOMBS)|g' \ -e 's|@''REPLACE_WCWIDTH''@|$(REPLACE_WCWIDTH)|g' \ -e 's|@''REPLACE_WCSWIDTH''@|$(REPLACE_WCSWIDTH)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. wctype.h: wctype.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's/@''HAVE_WCTYPE_H''@/$(HAVE_WCTYPE_H)/g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_WCTYPE_H''@|$(NEXT_WCTYPE_H)|g' \ -e 's/@''GNULIB_ISWBLANK''@/$(GNULIB_ISWBLANK)/g' \ -e 's/@''GNULIB_WCTYPE''@/$(GNULIB_WCTYPE)/g' \ -e 's/@''GNULIB_ISWCTYPE''@/$(GNULIB_ISWCTYPE)/g' \ -e 's/@''GNULIB_WCTRANS''@/$(GNULIB_WCTRANS)/g' \ -e 's/@''GNULIB_TOWCTRANS''@/$(GNULIB_TOWCTRANS)/g' \ -e 's/@''HAVE_ISWBLANK''@/$(HAVE_ISWBLANK)/g' \ -e 's/@''HAVE_ISWCNTRL''@/$(HAVE_ISWCNTRL)/g' \ -e 's/@''HAVE_WCTYPE_T''@/$(HAVE_WCTYPE_T)/g' \ -e 's/@''HAVE_WCTRANS_T''@/$(HAVE_WCTRANS_T)/g' \ -e 's/@''HAVE_WINT_T''@/$(HAVE_WINT_T)/g' \ -e 's/@''REPLACE_ISWBLANK''@/$(REPLACE_ISWBLANK)/g' \ -e 's/@''REPLACE_ISWCNTRL''@/$(REPLACE_ISWCNTRL)/g' \ -e 's/@''REPLACE_TOWLOWER''@/$(REPLACE_TOWLOWER)/g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/wctype.in.h; \ } > $@-t && \ mv $@-t $@ mostlyclean-local: mostlyclean-generic @for dir in '' $(MOSTLYCLEANDIRS); do \ if test -n "$$dir" && test -d $$dir; then \ echo "rmdir $$dir"; rmdir $$dir; \ fi; \ done; \ : # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: gnuastro-0.2.33-8a3b/bootstrapped/lib/Makefile.am0000644000175000017500000023441513004436760016441 00000000000000## DO NOT EDIT! GENERATED AUTOMATICALLY! ## Process this file with automake to produce Makefile.in. # Copyright (C) 2002-2016 Free Software Foundation, Inc. # # This file is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This file is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this file. If not, see . # # As a special exception to the GNU General Public License, # this file may be distributed as part of a program that # contains a configuration script generated by Autoconf, under # the same distribution terms as the rest of that program. # # Generated by gnulib-tool. # Reproduce by: gnulib-tool --import --local-dir=gl --lib=libgnu --source-base=bootstrapped/lib --m4-base=bootstrapped/m4 --doc-base=bootstrapped/doc --tests-base=bootstrapped/tests --aux-dir=bootstrapped/build-aux --with-tests --no-conditional-dependencies --libtool --macro-prefix=gl --no-vc-files argp error fdl gendocs git-version-gen math nproc regex strcase AUTOMAKE_OPTIONS = 1.9.6 gnits subdir-objects SUBDIRS = noinst_HEADERS = noinst_LIBRARIES = noinst_LTLIBRARIES = EXTRA_DIST = BUILT_SOURCES = SUFFIXES = MOSTLYCLEANFILES = core *.stackdump MOSTLYCLEANDIRS = CLEANFILES = DISTCLEANFILES = MAINTAINERCLEANFILES = AM_CPPFLAGS = AM_CFLAGS = noinst_LTLIBRARIES += libgnu.la libgnu_la_SOURCES = libgnu_la_LIBADD = $(gl_LTLIBOBJS) libgnu_la_DEPENDENCIES = $(gl_LTLIBOBJS) EXTRA_libgnu_la_SOURCES = libgnu_la_LDFLAGS = $(AM_LDFLAGS) libgnu_la_LDFLAGS += -no-undefined libgnu_la_LDFLAGS += $(LTLIBINTL) libgnu_la_LDFLAGS += $(LTLIBTHREAD) ## begin gnulib module absolute-header # Use this preprocessor expression to decide whether #include_next works. # Do not rely on a 'configure'-time test for this, since the expression # might appear in an installed header, which is used by some other compiler. HAVE_INCLUDE_NEXT = (__GNUC__ || 60000000 <= __DECC_VER) ## end gnulib module absolute-header ## begin gnulib module alloca libgnu_la_LIBADD += @LTALLOCA@ libgnu_la_DEPENDENCIES += @LTALLOCA@ EXTRA_DIST += alloca.c EXTRA_libgnu_la_SOURCES += alloca.c ## end gnulib module alloca ## begin gnulib module alloca-opt BUILT_SOURCES += $(ALLOCA_H) # We need the following in order to create when the system # doesn't have one that works with the given compiler. if GL_GENERATE_ALLOCA_H alloca.h: alloca.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ cat $(srcdir)/alloca.in.h; \ } > $@-t && \ mv -f $@-t $@ else alloca.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += alloca.h alloca.h-t EXTRA_DIST += alloca.in.h ## end gnulib module alloca-opt ## begin gnulib module argp libgnu_la_SOURCES += argp.h argp-ba.c argp-eexst.c argp-fmtstream.c argp-fmtstream.h argp-fs-xinl.c argp-help.c argp-namefrob.h argp-parse.c argp-pin.c argp-pv.c argp-pvh.c argp-xinl.c ## end gnulib module argp ## begin gnulib module btowc EXTRA_DIST += btowc.c EXTRA_libgnu_la_SOURCES += btowc.c ## end gnulib module btowc ## begin gnulib module c-ctype libgnu_la_SOURCES += c-ctype.h c-ctype.c ## end gnulib module c-ctype ## begin gnulib module configmake # Listed in the same order as the GNU makefile conventions, and # provided by autoconf 2.59c+ or 2.70. # The Automake-defined pkg* macros are appended, in the order # listed in the Automake 1.10a+ documentation. configmake.h: Makefile $(AM_V_GEN)rm -f $@-t && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ echo '#define PREFIX "$(prefix)"'; \ echo '#define EXEC_PREFIX "$(exec_prefix)"'; \ echo '#define BINDIR "$(bindir)"'; \ echo '#define SBINDIR "$(sbindir)"'; \ echo '#define LIBEXECDIR "$(libexecdir)"'; \ echo '#define DATAROOTDIR "$(datarootdir)"'; \ echo '#define DATADIR "$(datadir)"'; \ echo '#define SYSCONFDIR "$(sysconfdir)"'; \ echo '#define SHAREDSTATEDIR "$(sharedstatedir)"'; \ echo '#define LOCALSTATEDIR "$(localstatedir)"'; \ echo '#define RUNSTATEDIR "$(runstatedir)"'; \ echo '#define INCLUDEDIR "$(includedir)"'; \ echo '#define OLDINCLUDEDIR "$(oldincludedir)"'; \ echo '#define DOCDIR "$(docdir)"'; \ echo '#define INFODIR "$(infodir)"'; \ echo '#define HTMLDIR "$(htmldir)"'; \ echo '#define DVIDIR "$(dvidir)"'; \ echo '#define PDFDIR "$(pdfdir)"'; \ echo '#define PSDIR "$(psdir)"'; \ echo '#define LIBDIR "$(libdir)"'; \ echo '#define LISPDIR "$(lispdir)"'; \ echo '#define LOCALEDIR "$(localedir)"'; \ echo '#define MANDIR "$(mandir)"'; \ echo '#define MANEXT "$(manext)"'; \ echo '#define PKGDATADIR "$(pkgdatadir)"'; \ echo '#define PKGINCLUDEDIR "$(pkgincludedir)"'; \ echo '#define PKGLIBDIR "$(pkglibdir)"'; \ echo '#define PKGLIBEXECDIR "$(pkglibexecdir)"'; \ } | sed '/""/d' > $@-t && \ mv -f $@-t $@ BUILT_SOURCES += configmake.h CLEANFILES += configmake.h configmake.h-t ## end gnulib module configmake ## begin gnulib module dirname-lgpl libgnu_la_SOURCES += dirname-lgpl.c basename-lgpl.c stripslash.c EXTRA_DIST += dirname.h ## end gnulib module dirname-lgpl ## begin gnulib module dosname EXTRA_DIST += dosname.h ## end gnulib module dosname ## begin gnulib module errno BUILT_SOURCES += $(ERRNO_H) # We need the following in order to create when the system # doesn't have one that is POSIX compliant. if GL_GENERATE_ERRNO_H errno.h: errno.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_ERRNO_H''@|$(NEXT_ERRNO_H)|g' \ -e 's|@''EMULTIHOP_HIDDEN''@|$(EMULTIHOP_HIDDEN)|g' \ -e 's|@''EMULTIHOP_VALUE''@|$(EMULTIHOP_VALUE)|g' \ -e 's|@''ENOLINK_HIDDEN''@|$(ENOLINK_HIDDEN)|g' \ -e 's|@''ENOLINK_VALUE''@|$(ENOLINK_VALUE)|g' \ -e 's|@''EOVERFLOW_HIDDEN''@|$(EOVERFLOW_HIDDEN)|g' \ -e 's|@''EOVERFLOW_VALUE''@|$(EOVERFLOW_VALUE)|g' \ < $(srcdir)/errno.in.h; \ } > $@-t && \ mv $@-t $@ else errno.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += errno.h errno.h-t EXTRA_DIST += errno.in.h ## end gnulib module errno ## begin gnulib module error EXTRA_DIST += error.c error.h EXTRA_libgnu_la_SOURCES += error.c ## end gnulib module error ## begin gnulib module float BUILT_SOURCES += $(FLOAT_H) # We need the following in order to create when the system # doesn't have one that works with the given compiler. if GL_GENERATE_FLOAT_H float.h: float.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_FLOAT_H''@|$(NEXT_FLOAT_H)|g' \ -e 's|@''REPLACE_ITOLD''@|$(REPLACE_ITOLD)|g' \ < $(srcdir)/float.in.h; \ } > $@-t && \ mv $@-t $@ else float.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += float.h float.h-t EXTRA_DIST += float.c float.in.h itold.c EXTRA_libgnu_la_SOURCES += float.c itold.c ## end gnulib module float ## begin gnulib module gendocs EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/gendocs.sh ## end gnulib module gendocs ## begin gnulib module getopt-posix BUILT_SOURCES += $(GETOPT_H) # We need the following in order to create when the system # doesn't have one that works with the given compiler. getopt.h: getopt.in.h $(top_builddir)/config.status $(ARG_NONNULL_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''HAVE_GETOPT_H''@|$(HAVE_GETOPT_H)|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_GETOPT_H''@|$(NEXT_GETOPT_H)|g' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ < $(srcdir)/getopt.in.h; \ } > $@-t && \ mv -f $@-t $@ MOSTLYCLEANFILES += getopt.h getopt.h-t EXTRA_DIST += getopt.c getopt.in.h getopt1.c getopt_int.h EXTRA_libgnu_la_SOURCES += getopt.c getopt1.c ## end gnulib module getopt-posix ## begin gnulib module getprogname libgnu_la_SOURCES += getprogname.h getprogname.c ## end gnulib module getprogname ## begin gnulib module gettext-h libgnu_la_SOURCES += gettext.h ## end gnulib module gettext-h ## begin gnulib module git-version-gen EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/git-version-gen ## end gnulib module git-version-gen ## begin gnulib module hard-locale libgnu_la_SOURCES += hard-locale.c EXTRA_DIST += hard-locale.h ## end gnulib module hard-locale ## begin gnulib module havelib EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/config.rpath ## end gnulib module havelib ## begin gnulib module intprops EXTRA_DIST += intprops.h ## end gnulib module intprops ## begin gnulib module langinfo BUILT_SOURCES += langinfo.h # We need the following in order to create an empty placeholder for # when the system doesn't have one. langinfo.h: langinfo.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''HAVE_LANGINFO_H''@|$(HAVE_LANGINFO_H)|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_LANGINFO_H''@|$(NEXT_LANGINFO_H)|g' \ -e 's/@''GNULIB_NL_LANGINFO''@/$(GNULIB_NL_LANGINFO)/g' \ -e 's|@''HAVE_LANGINFO_CODESET''@|$(HAVE_LANGINFO_CODESET)|g' \ -e 's|@''HAVE_LANGINFO_T_FMT_AMPM''@|$(HAVE_LANGINFO_T_FMT_AMPM)|g' \ -e 's|@''HAVE_LANGINFO_ERA''@|$(HAVE_LANGINFO_ERA)|g' \ -e 's|@''HAVE_LANGINFO_YESEXPR''@|$(HAVE_LANGINFO_YESEXPR)|g' \ -e 's|@''HAVE_NL_LANGINFO''@|$(HAVE_NL_LANGINFO)|g' \ -e 's|@''REPLACE_NL_LANGINFO''@|$(REPLACE_NL_LANGINFO)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/langinfo.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += langinfo.h langinfo.h-t EXTRA_DIST += langinfo.in.h ## end gnulib module langinfo ## begin gnulib module limits-h BUILT_SOURCES += $(LIMITS_H) # We need the following in order to create when the system # doesn't have one that is compatible with GNU. if GL_GENERATE_LIMITS_H limits.h: limits.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_LIMITS_H''@|$(NEXT_LIMITS_H)|g' \ < $(srcdir)/limits.in.h; \ } > $@-t && \ mv $@-t $@ else limits.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += limits.h limits.h-t EXTRA_DIST += limits.in.h ## end gnulib module limits-h ## begin gnulib module localcharset libgnu_la_SOURCES += localcharset.h localcharset.c # We need the following in order to install a simple file in $(libdir) # which is shared with other installed packages. We use a list of referencing # packages so that "make uninstall" will remove the file if and only if it # is not used by another installed package. # On systems with glibc-2.1 or newer, the file is redundant, therefore we # avoid installing it. all-local: charset.alias ref-add.sed ref-del.sed charset_alias = $(DESTDIR)$(libdir)/charset.alias charset_tmp = $(DESTDIR)$(libdir)/charset.tmp install-exec-local: install-exec-localcharset install-exec-localcharset: all-local if test $(GLIBC21) = no; then \ case '$(host_os)' in \ darwin[56]*) \ need_charset_alias=true ;; \ darwin* | cygwin* | mingw* | pw32* | cegcc*) \ need_charset_alias=false ;; \ *) \ need_charset_alias=true ;; \ esac ; \ else \ need_charset_alias=false ; \ fi ; \ if $$need_charset_alias; then \ $(mkinstalldirs) $(DESTDIR)$(libdir) ; \ fi ; \ if test -f $(charset_alias); then \ sed -f ref-add.sed $(charset_alias) > $(charset_tmp) ; \ $(INSTALL_DATA) $(charset_tmp) $(charset_alias) ; \ rm -f $(charset_tmp) ; \ else \ if $$need_charset_alias; then \ sed -f ref-add.sed charset.alias > $(charset_tmp) ; \ $(INSTALL_DATA) $(charset_tmp) $(charset_alias) ; \ rm -f $(charset_tmp) ; \ fi ; \ fi uninstall-local: uninstall-localcharset uninstall-localcharset: all-local if test -f $(charset_alias); then \ sed -f ref-del.sed $(charset_alias) > $(charset_tmp); \ if grep '^# Packages using this file: $$' $(charset_tmp) \ > /dev/null; then \ rm -f $(charset_alias); \ else \ $(INSTALL_DATA) $(charset_tmp) $(charset_alias); \ fi; \ rm -f $(charset_tmp); \ fi charset.alias: config.charset $(AM_V_GEN)rm -f t-$@ $@ && \ $(SHELL) $(srcdir)/config.charset '$(host)' > t-$@ && \ mv t-$@ $@ SUFFIXES += .sed .sin .sin.sed: $(AM_V_GEN)rm -f t-$@ $@ && \ sed -e '/^#/d' -e 's/@''PACKAGE''@/$(PACKAGE)/g' $< > t-$@ && \ mv t-$@ $@ CLEANFILES += charset.alias ref-add.sed ref-del.sed EXTRA_DIST += config.charset ref-add.sin ref-del.sin ## end gnulib module localcharset ## begin gnulib module locale BUILT_SOURCES += locale.h # We need the following in order to create when the system # doesn't have one that provides all definitions. locale.h: locale.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_LOCALE_H''@|$(NEXT_LOCALE_H)|g' \ -e 's/@''GNULIB_LOCALECONV''@/$(GNULIB_LOCALECONV)/g' \ -e 's/@''GNULIB_SETLOCALE''@/$(GNULIB_SETLOCALE)/g' \ -e 's/@''GNULIB_DUPLOCALE''@/$(GNULIB_DUPLOCALE)/g' \ -e 's|@''HAVE_DUPLOCALE''@|$(HAVE_DUPLOCALE)|g' \ -e 's|@''HAVE_XLOCALE_H''@|$(HAVE_XLOCALE_H)|g' \ -e 's|@''REPLACE_LOCALECONV''@|$(REPLACE_LOCALECONV)|g' \ -e 's|@''REPLACE_SETLOCALE''@|$(REPLACE_SETLOCALE)|g' \ -e 's|@''REPLACE_DUPLOCALE''@|$(REPLACE_DUPLOCALE)|g' \ -e 's|@''REPLACE_STRUCT_LCONV''@|$(REPLACE_STRUCT_LCONV)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/locale.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += locale.h locale.h-t EXTRA_DIST += locale.in.h ## end gnulib module locale ## begin gnulib module localeconv EXTRA_DIST += localeconv.c EXTRA_libgnu_la_SOURCES += localeconv.c ## end gnulib module localeconv ## begin gnulib module lock libgnu_la_SOURCES += glthread/lock.h glthread/lock.c ## end gnulib module lock ## begin gnulib module malloc-gnu EXTRA_DIST += malloc.c EXTRA_libgnu_la_SOURCES += malloc.c ## end gnulib module malloc-gnu ## begin gnulib module malloc-posix EXTRA_DIST += malloc.c EXTRA_libgnu_la_SOURCES += malloc.c ## end gnulib module malloc-posix ## begin gnulib module math BUILT_SOURCES += math.h libgnu_la_SOURCES += math.c # We need the following in order to create when the system # doesn't have one that works with the given compiler. math.h: math.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT_AS_FIRST_DIRECTIVE''@|$(INCLUDE_NEXT_AS_FIRST_DIRECTIVE)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_AS_FIRST_DIRECTIVE_MATH_H''@|$(NEXT_AS_FIRST_DIRECTIVE_MATH_H)|g' \ -e 's/@''GNULIB_ACOSF''@/$(GNULIB_ACOSF)/g' \ -e 's/@''GNULIB_ACOSL''@/$(GNULIB_ACOSL)/g' \ -e 's/@''GNULIB_ASINF''@/$(GNULIB_ASINF)/g' \ -e 's/@''GNULIB_ASINL''@/$(GNULIB_ASINL)/g' \ -e 's/@''GNULIB_ATANF''@/$(GNULIB_ATANF)/g' \ -e 's/@''GNULIB_ATANL''@/$(GNULIB_ATANL)/g' \ -e 's/@''GNULIB_ATAN2F''@/$(GNULIB_ATAN2F)/g' \ -e 's/@''GNULIB_CBRT''@/$(GNULIB_CBRT)/g' \ -e 's/@''GNULIB_CBRTF''@/$(GNULIB_CBRTF)/g' \ -e 's/@''GNULIB_CBRTL''@/$(GNULIB_CBRTL)/g' \ -e 's/@''GNULIB_CEIL''@/$(GNULIB_CEIL)/g' \ -e 's/@''GNULIB_CEILF''@/$(GNULIB_CEILF)/g' \ -e 's/@''GNULIB_CEILL''@/$(GNULIB_CEILL)/g' \ -e 's/@''GNULIB_COPYSIGN''@/$(GNULIB_COPYSIGN)/g' \ -e 's/@''GNULIB_COPYSIGNF''@/$(GNULIB_COPYSIGNF)/g' \ -e 's/@''GNULIB_COPYSIGNL''@/$(GNULIB_COPYSIGNL)/g' \ -e 's/@''GNULIB_COSF''@/$(GNULIB_COSF)/g' \ -e 's/@''GNULIB_COSL''@/$(GNULIB_COSL)/g' \ -e 's/@''GNULIB_COSHF''@/$(GNULIB_COSHF)/g' \ -e 's/@''GNULIB_EXPF''@/$(GNULIB_EXPF)/g' \ -e 's/@''GNULIB_EXPL''@/$(GNULIB_EXPL)/g' \ -e 's/@''GNULIB_EXP2''@/$(GNULIB_EXP2)/g' \ -e 's/@''GNULIB_EXP2F''@/$(GNULIB_EXP2F)/g' \ -e 's/@''GNULIB_EXP2L''@/$(GNULIB_EXP2L)/g' \ -e 's/@''GNULIB_EXPM1''@/$(GNULIB_EXPM1)/g' \ -e 's/@''GNULIB_EXPM1F''@/$(GNULIB_EXPM1F)/g' \ -e 's/@''GNULIB_EXPM1L''@/$(GNULIB_EXPM1L)/g' \ -e 's/@''GNULIB_FABSF''@/$(GNULIB_FABSF)/g' \ -e 's/@''GNULIB_FABSL''@/$(GNULIB_FABSL)/g' \ -e 's/@''GNULIB_FLOOR''@/$(GNULIB_FLOOR)/g' \ -e 's/@''GNULIB_FLOORF''@/$(GNULIB_FLOORF)/g' \ -e 's/@''GNULIB_FLOORL''@/$(GNULIB_FLOORL)/g' \ -e 's/@''GNULIB_FMA''@/$(GNULIB_FMA)/g' \ -e 's/@''GNULIB_FMAF''@/$(GNULIB_FMAF)/g' \ -e 's/@''GNULIB_FMAL''@/$(GNULIB_FMAL)/g' \ -e 's/@''GNULIB_FMOD''@/$(GNULIB_FMOD)/g' \ -e 's/@''GNULIB_FMODF''@/$(GNULIB_FMODF)/g' \ -e 's/@''GNULIB_FMODL''@/$(GNULIB_FMODL)/g' \ -e 's/@''GNULIB_FREXPF''@/$(GNULIB_FREXPF)/g' \ -e 's/@''GNULIB_FREXP''@/$(GNULIB_FREXP)/g' \ -e 's/@''GNULIB_FREXPL''@/$(GNULIB_FREXPL)/g' \ -e 's/@''GNULIB_HYPOT''@/$(GNULIB_HYPOT)/g' \ -e 's/@''GNULIB_HYPOTF''@/$(GNULIB_HYPOTF)/g' \ -e 's/@''GNULIB_HYPOTL''@/$(GNULIB_HYPOTL)/g' \ < $(srcdir)/math.in.h | \ sed -e 's/@''GNULIB_ILOGB''@/$(GNULIB_ILOGB)/g' \ -e 's/@''GNULIB_ILOGBF''@/$(GNULIB_ILOGBF)/g' \ -e 's/@''GNULIB_ILOGBL''@/$(GNULIB_ILOGBL)/g' \ -e 's/@''GNULIB_ISFINITE''@/$(GNULIB_ISFINITE)/g' \ -e 's/@''GNULIB_ISINF''@/$(GNULIB_ISINF)/g' \ -e 's/@''GNULIB_ISNAN''@/$(GNULIB_ISNAN)/g' \ -e 's/@''GNULIB_ISNANF''@/$(GNULIB_ISNANF)/g' \ -e 's/@''GNULIB_ISNAND''@/$(GNULIB_ISNAND)/g' \ -e 's/@''GNULIB_ISNANL''@/$(GNULIB_ISNANL)/g' \ -e 's/@''GNULIB_LDEXPF''@/$(GNULIB_LDEXPF)/g' \ -e 's/@''GNULIB_LDEXPL''@/$(GNULIB_LDEXPL)/g' \ -e 's/@''GNULIB_LOG''@/$(GNULIB_LOG)/g' \ -e 's/@''GNULIB_LOGF''@/$(GNULIB_LOGF)/g' \ -e 's/@''GNULIB_LOGL''@/$(GNULIB_LOGL)/g' \ -e 's/@''GNULIB_LOG10''@/$(GNULIB_LOG10)/g' \ -e 's/@''GNULIB_LOG10F''@/$(GNULIB_LOG10F)/g' \ -e 's/@''GNULIB_LOG10L''@/$(GNULIB_LOG10L)/g' \ -e 's/@''GNULIB_LOG1P''@/$(GNULIB_LOG1P)/g' \ -e 's/@''GNULIB_LOG1PF''@/$(GNULIB_LOG1PF)/g' \ -e 's/@''GNULIB_LOG1PL''@/$(GNULIB_LOG1PL)/g' \ -e 's/@''GNULIB_LOG2''@/$(GNULIB_LOG2)/g' \ -e 's/@''GNULIB_LOG2F''@/$(GNULIB_LOG2F)/g' \ -e 's/@''GNULIB_LOG2L''@/$(GNULIB_LOG2L)/g' \ -e 's/@''GNULIB_LOGB''@/$(GNULIB_LOGB)/g' \ -e 's/@''GNULIB_LOGBF''@/$(GNULIB_LOGBF)/g' \ -e 's/@''GNULIB_LOGBL''@/$(GNULIB_LOGBL)/g' \ -e 's/@''GNULIB_MODF''@/$(GNULIB_MODF)/g' \ -e 's/@''GNULIB_MODFF''@/$(GNULIB_MODFF)/g' \ -e 's/@''GNULIB_MODFL''@/$(GNULIB_MODFL)/g' \ -e 's/@''GNULIB_POWF''@/$(GNULIB_POWF)/g' \ -e 's/@''GNULIB_REMAINDER''@/$(GNULIB_REMAINDER)/g' \ -e 's/@''GNULIB_REMAINDERF''@/$(GNULIB_REMAINDERF)/g' \ -e 's/@''GNULIB_REMAINDERL''@/$(GNULIB_REMAINDERL)/g' \ -e 's/@''GNULIB_RINT''@/$(GNULIB_RINT)/g' \ -e 's/@''GNULIB_RINTF''@/$(GNULIB_RINTF)/g' \ -e 's/@''GNULIB_RINTL''@/$(GNULIB_RINTL)/g' \ -e 's/@''GNULIB_ROUND''@/$(GNULIB_ROUND)/g' \ -e 's/@''GNULIB_ROUNDF''@/$(GNULIB_ROUNDF)/g' \ -e 's/@''GNULIB_ROUNDL''@/$(GNULIB_ROUNDL)/g' \ -e 's/@''GNULIB_SIGNBIT''@/$(GNULIB_SIGNBIT)/g' \ -e 's/@''GNULIB_SINF''@/$(GNULIB_SINF)/g' \ -e 's/@''GNULIB_SINL''@/$(GNULIB_SINL)/g' \ -e 's/@''GNULIB_SINHF''@/$(GNULIB_SINHF)/g' \ -e 's/@''GNULIB_SQRTF''@/$(GNULIB_SQRTF)/g' \ -e 's/@''GNULIB_SQRTL''@/$(GNULIB_SQRTL)/g' \ -e 's/@''GNULIB_TANF''@/$(GNULIB_TANF)/g' \ -e 's/@''GNULIB_TANL''@/$(GNULIB_TANL)/g' \ -e 's/@''GNULIB_TANHF''@/$(GNULIB_TANHF)/g' \ -e 's/@''GNULIB_TRUNC''@/$(GNULIB_TRUNC)/g' \ -e 's/@''GNULIB_TRUNCF''@/$(GNULIB_TRUNCF)/g' \ -e 's/@''GNULIB_TRUNCL''@/$(GNULIB_TRUNCL)/g' \ | \ sed -e 's|@''HAVE_ACOSF''@|$(HAVE_ACOSF)|g' \ -e 's|@''HAVE_ACOSL''@|$(HAVE_ACOSL)|g' \ -e 's|@''HAVE_ASINF''@|$(HAVE_ASINF)|g' \ -e 's|@''HAVE_ASINL''@|$(HAVE_ASINL)|g' \ -e 's|@''HAVE_ATANF''@|$(HAVE_ATANF)|g' \ -e 's|@''HAVE_ATANL''@|$(HAVE_ATANL)|g' \ -e 's|@''HAVE_ATAN2F''@|$(HAVE_ATAN2F)|g' \ -e 's|@''HAVE_CBRT''@|$(HAVE_CBRT)|g' \ -e 's|@''HAVE_CBRTF''@|$(HAVE_CBRTF)|g' \ -e 's|@''HAVE_CBRTL''@|$(HAVE_CBRTL)|g' \ -e 's|@''HAVE_COPYSIGN''@|$(HAVE_COPYSIGN)|g' \ -e 's|@''HAVE_COPYSIGNL''@|$(HAVE_COPYSIGNL)|g' \ -e 's|@''HAVE_COSF''@|$(HAVE_COSF)|g' \ -e 's|@''HAVE_COSL''@|$(HAVE_COSL)|g' \ -e 's|@''HAVE_COSHF''@|$(HAVE_COSHF)|g' \ -e 's|@''HAVE_EXPF''@|$(HAVE_EXPF)|g' \ -e 's|@''HAVE_EXPL''@|$(HAVE_EXPL)|g' \ -e 's|@''HAVE_EXPM1''@|$(HAVE_EXPM1)|g' \ -e 's|@''HAVE_EXPM1F''@|$(HAVE_EXPM1F)|g' \ -e 's|@''HAVE_FABSF''@|$(HAVE_FABSF)|g' \ -e 's|@''HAVE_FABSL''@|$(HAVE_FABSL)|g' \ -e 's|@''HAVE_FMA''@|$(HAVE_FMA)|g' \ -e 's|@''HAVE_FMAF''@|$(HAVE_FMAF)|g' \ -e 's|@''HAVE_FMAL''@|$(HAVE_FMAL)|g' \ -e 's|@''HAVE_FMODF''@|$(HAVE_FMODF)|g' \ -e 's|@''HAVE_FMODL''@|$(HAVE_FMODL)|g' \ -e 's|@''HAVE_FREXPF''@|$(HAVE_FREXPF)|g' \ -e 's|@''HAVE_HYPOTF''@|$(HAVE_HYPOTF)|g' \ -e 's|@''HAVE_HYPOTL''@|$(HAVE_HYPOTL)|g' \ -e 's|@''HAVE_ILOGB''@|$(HAVE_ILOGB)|g' \ -e 's|@''HAVE_ILOGBF''@|$(HAVE_ILOGBF)|g' \ -e 's|@''HAVE_ILOGBL''@|$(HAVE_ILOGBL)|g' \ -e 's|@''HAVE_ISNANF''@|$(HAVE_ISNANF)|g' \ -e 's|@''HAVE_ISNAND''@|$(HAVE_ISNAND)|g' \ -e 's|@''HAVE_ISNANL''@|$(HAVE_ISNANL)|g' \ -e 's|@''HAVE_LDEXPF''@|$(HAVE_LDEXPF)|g' \ -e 's|@''HAVE_LOGF''@|$(HAVE_LOGF)|g' \ -e 's|@''HAVE_LOGL''@|$(HAVE_LOGL)|g' \ -e 's|@''HAVE_LOG10F''@|$(HAVE_LOG10F)|g' \ -e 's|@''HAVE_LOG10L''@|$(HAVE_LOG10L)|g' \ -e 's|@''HAVE_LOG1P''@|$(HAVE_LOG1P)|g' \ -e 's|@''HAVE_LOG1PF''@|$(HAVE_LOG1PF)|g' \ -e 's|@''HAVE_LOG1PL''@|$(HAVE_LOG1PL)|g' \ -e 's|@''HAVE_LOGBF''@|$(HAVE_LOGBF)|g' \ -e 's|@''HAVE_LOGBL''@|$(HAVE_LOGBL)|g' \ -e 's|@''HAVE_MODFF''@|$(HAVE_MODFF)|g' \ -e 's|@''HAVE_MODFL''@|$(HAVE_MODFL)|g' \ -e 's|@''HAVE_POWF''@|$(HAVE_POWF)|g' \ -e 's|@''HAVE_REMAINDER''@|$(HAVE_REMAINDER)|g' \ -e 's|@''HAVE_REMAINDERF''@|$(HAVE_REMAINDERF)|g' \ -e 's|@''HAVE_RINT''@|$(HAVE_RINT)|g' \ -e 's|@''HAVE_RINTL''@|$(HAVE_RINTL)|g' \ -e 's|@''HAVE_SINF''@|$(HAVE_SINF)|g' \ -e 's|@''HAVE_SINL''@|$(HAVE_SINL)|g' \ -e 's|@''HAVE_SINHF''@|$(HAVE_SINHF)|g' \ -e 's|@''HAVE_SQRTF''@|$(HAVE_SQRTF)|g' \ -e 's|@''HAVE_SQRTL''@|$(HAVE_SQRTL)|g' \ -e 's|@''HAVE_TANF''@|$(HAVE_TANF)|g' \ -e 's|@''HAVE_TANL''@|$(HAVE_TANL)|g' \ -e 's|@''HAVE_TANHF''@|$(HAVE_TANHF)|g' \ -e 's|@''HAVE_DECL_ACOSL''@|$(HAVE_DECL_ACOSL)|g' \ -e 's|@''HAVE_DECL_ASINL''@|$(HAVE_DECL_ASINL)|g' \ -e 's|@''HAVE_DECL_ATANL''@|$(HAVE_DECL_ATANL)|g' \ -e 's|@''HAVE_DECL_CBRTF''@|$(HAVE_DECL_CBRTF)|g' \ -e 's|@''HAVE_DECL_CBRTL''@|$(HAVE_DECL_CBRTL)|g' \ -e 's|@''HAVE_DECL_CEILF''@|$(HAVE_DECL_CEILF)|g' \ -e 's|@''HAVE_DECL_CEILL''@|$(HAVE_DECL_CEILL)|g' \ -e 's|@''HAVE_DECL_COPYSIGNF''@|$(HAVE_DECL_COPYSIGNF)|g' \ -e 's|@''HAVE_DECL_COSL''@|$(HAVE_DECL_COSL)|g' \ -e 's|@''HAVE_DECL_EXPL''@|$(HAVE_DECL_EXPL)|g' \ -e 's|@''HAVE_DECL_EXP2''@|$(HAVE_DECL_EXP2)|g' \ -e 's|@''HAVE_DECL_EXP2F''@|$(HAVE_DECL_EXP2F)|g' \ -e 's|@''HAVE_DECL_EXP2L''@|$(HAVE_DECL_EXP2L)|g' \ -e 's|@''HAVE_DECL_EXPM1L''@|$(HAVE_DECL_EXPM1L)|g' \ -e 's|@''HAVE_DECL_FLOORF''@|$(HAVE_DECL_FLOORF)|g' \ -e 's|@''HAVE_DECL_FLOORL''@|$(HAVE_DECL_FLOORL)|g' \ -e 's|@''HAVE_DECL_FREXPL''@|$(HAVE_DECL_FREXPL)|g' \ -e 's|@''HAVE_DECL_LDEXPL''@|$(HAVE_DECL_LDEXPL)|g' \ -e 's|@''HAVE_DECL_LOGL''@|$(HAVE_DECL_LOGL)|g' \ -e 's|@''HAVE_DECL_LOG10L''@|$(HAVE_DECL_LOG10L)|g' \ -e 's|@''HAVE_DECL_LOG2''@|$(HAVE_DECL_LOG2)|g' \ -e 's|@''HAVE_DECL_LOG2F''@|$(HAVE_DECL_LOG2F)|g' \ -e 's|@''HAVE_DECL_LOG2L''@|$(HAVE_DECL_LOG2L)|g' \ -e 's|@''HAVE_DECL_LOGB''@|$(HAVE_DECL_LOGB)|g' \ -e 's|@''HAVE_DECL_REMAINDER''@|$(HAVE_DECL_REMAINDER)|g' \ -e 's|@''HAVE_DECL_REMAINDERL''@|$(HAVE_DECL_REMAINDERL)|g' \ -e 's|@''HAVE_DECL_RINTF''@|$(HAVE_DECL_RINTF)|g' \ -e 's|@''HAVE_DECL_ROUND''@|$(HAVE_DECL_ROUND)|g' \ -e 's|@''HAVE_DECL_ROUNDF''@|$(HAVE_DECL_ROUNDF)|g' \ -e 's|@''HAVE_DECL_ROUNDL''@|$(HAVE_DECL_ROUNDL)|g' \ -e 's|@''HAVE_DECL_SINL''@|$(HAVE_DECL_SINL)|g' \ -e 's|@''HAVE_DECL_SQRTL''@|$(HAVE_DECL_SQRTL)|g' \ -e 's|@''HAVE_DECL_TANL''@|$(HAVE_DECL_TANL)|g' \ -e 's|@''HAVE_DECL_TRUNC''@|$(HAVE_DECL_TRUNC)|g' \ -e 's|@''HAVE_DECL_TRUNCF''@|$(HAVE_DECL_TRUNCF)|g' \ -e 's|@''HAVE_DECL_TRUNCL''@|$(HAVE_DECL_TRUNCL)|g' \ | \ sed -e 's|@''REPLACE_CBRTF''@|$(REPLACE_CBRTF)|g' \ -e 's|@''REPLACE_CBRTL''@|$(REPLACE_CBRTL)|g' \ -e 's|@''REPLACE_CEIL''@|$(REPLACE_CEIL)|g' \ -e 's|@''REPLACE_CEILF''@|$(REPLACE_CEILF)|g' \ -e 's|@''REPLACE_CEILL''@|$(REPLACE_CEILL)|g' \ -e 's|@''REPLACE_EXPM1''@|$(REPLACE_EXPM1)|g' \ -e 's|@''REPLACE_EXPM1F''@|$(REPLACE_EXPM1F)|g' \ -e 's|@''REPLACE_EXP2''@|$(REPLACE_EXP2)|g' \ -e 's|@''REPLACE_EXP2L''@|$(REPLACE_EXP2L)|g' \ -e 's|@''REPLACE_FABSL''@|$(REPLACE_FABSL)|g' \ -e 's|@''REPLACE_FLOOR''@|$(REPLACE_FLOOR)|g' \ -e 's|@''REPLACE_FLOORF''@|$(REPLACE_FLOORF)|g' \ -e 's|@''REPLACE_FLOORL''@|$(REPLACE_FLOORL)|g' \ -e 's|@''REPLACE_FMA''@|$(REPLACE_FMA)|g' \ -e 's|@''REPLACE_FMAF''@|$(REPLACE_FMAF)|g' \ -e 's|@''REPLACE_FMAL''@|$(REPLACE_FMAL)|g' \ -e 's|@''REPLACE_FMOD''@|$(REPLACE_FMOD)|g' \ -e 's|@''REPLACE_FMODF''@|$(REPLACE_FMODF)|g' \ -e 's|@''REPLACE_FMODL''@|$(REPLACE_FMODL)|g' \ -e 's|@''REPLACE_FREXPF''@|$(REPLACE_FREXPF)|g' \ -e 's|@''REPLACE_FREXP''@|$(REPLACE_FREXP)|g' \ -e 's|@''REPLACE_FREXPL''@|$(REPLACE_FREXPL)|g' \ -e 's|@''REPLACE_HUGE_VAL''@|$(REPLACE_HUGE_VAL)|g' \ -e 's|@''REPLACE_HYPOT''@|$(REPLACE_HYPOT)|g' \ -e 's|@''REPLACE_HYPOTF''@|$(REPLACE_HYPOTF)|g' \ -e 's|@''REPLACE_HYPOTL''@|$(REPLACE_HYPOTL)|g' \ -e 's|@''REPLACE_ILOGB''@|$(REPLACE_ILOGB)|g' \ -e 's|@''REPLACE_ILOGBF''@|$(REPLACE_ILOGBF)|g' \ -e 's|@''REPLACE_ISFINITE''@|$(REPLACE_ISFINITE)|g' \ -e 's|@''REPLACE_ISINF''@|$(REPLACE_ISINF)|g' \ -e 's|@''REPLACE_ISNAN''@|$(REPLACE_ISNAN)|g' \ -e 's|@''REPLACE_ITOLD''@|$(REPLACE_ITOLD)|g' \ -e 's|@''REPLACE_LDEXPL''@|$(REPLACE_LDEXPL)|g' \ -e 's|@''REPLACE_LOG''@|$(REPLACE_LOG)|g' \ -e 's|@''REPLACE_LOGF''@|$(REPLACE_LOGF)|g' \ -e 's|@''REPLACE_LOGL''@|$(REPLACE_LOGL)|g' \ -e 's|@''REPLACE_LOG10''@|$(REPLACE_LOG10)|g' \ -e 's|@''REPLACE_LOG10F''@|$(REPLACE_LOG10F)|g' \ -e 's|@''REPLACE_LOG10L''@|$(REPLACE_LOG10L)|g' \ -e 's|@''REPLACE_LOG1P''@|$(REPLACE_LOG1P)|g' \ -e 's|@''REPLACE_LOG1PF''@|$(REPLACE_LOG1PF)|g' \ -e 's|@''REPLACE_LOG1PL''@|$(REPLACE_LOG1PL)|g' \ -e 's|@''REPLACE_LOG2''@|$(REPLACE_LOG2)|g' \ -e 's|@''REPLACE_LOG2F''@|$(REPLACE_LOG2F)|g' \ -e 's|@''REPLACE_LOG2L''@|$(REPLACE_LOG2L)|g' \ -e 's|@''REPLACE_LOGB''@|$(REPLACE_LOGB)|g' \ -e 's|@''REPLACE_LOGBF''@|$(REPLACE_LOGBF)|g' \ -e 's|@''REPLACE_LOGBL''@|$(REPLACE_LOGBL)|g' \ -e 's|@''REPLACE_MODF''@|$(REPLACE_MODF)|g' \ -e 's|@''REPLACE_MODFF''@|$(REPLACE_MODFF)|g' \ -e 's|@''REPLACE_MODFL''@|$(REPLACE_MODFL)|g' \ -e 's|@''REPLACE_NAN''@|$(REPLACE_NAN)|g' \ -e 's|@''REPLACE_REMAINDER''@|$(REPLACE_REMAINDER)|g' \ -e 's|@''REPLACE_REMAINDERF''@|$(REPLACE_REMAINDERF)|g' \ -e 's|@''REPLACE_REMAINDERL''@|$(REPLACE_REMAINDERL)|g' \ -e 's|@''REPLACE_ROUND''@|$(REPLACE_ROUND)|g' \ -e 's|@''REPLACE_ROUNDF''@|$(REPLACE_ROUNDF)|g' \ -e 's|@''REPLACE_ROUNDL''@|$(REPLACE_ROUNDL)|g' \ -e 's|@''REPLACE_SIGNBIT''@|$(REPLACE_SIGNBIT)|g' \ -e 's|@''REPLACE_SIGNBIT_USING_GCC''@|$(REPLACE_SIGNBIT_USING_GCC)|g' \ -e 's|@''REPLACE_SQRTL''@|$(REPLACE_SQRTL)|g' \ -e 's|@''REPLACE_TRUNC''@|$(REPLACE_TRUNC)|g' \ -e 's|@''REPLACE_TRUNCF''@|$(REPLACE_TRUNCF)|g' \ -e 's|@''REPLACE_TRUNCL''@|$(REPLACE_TRUNCL)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += math.h math.h-t EXTRA_DIST += math.in.h ## end gnulib module math ## begin gnulib module mbrtowc EXTRA_DIST += mbrtowc.c EXTRA_libgnu_la_SOURCES += mbrtowc.c ## end gnulib module mbrtowc ## begin gnulib module mbsinit EXTRA_DIST += mbsinit.c EXTRA_libgnu_la_SOURCES += mbsinit.c ## end gnulib module mbsinit ## begin gnulib module mbtowc EXTRA_DIST += mbtowc-impl.h mbtowc.c EXTRA_libgnu_la_SOURCES += mbtowc.c ## end gnulib module mbtowc ## begin gnulib module memchr EXTRA_DIST += memchr.c memchr.valgrind EXTRA_libgnu_la_SOURCES += memchr.c ## end gnulib module memchr ## begin gnulib module mempcpy EXTRA_DIST += mempcpy.c EXTRA_libgnu_la_SOURCES += mempcpy.c ## end gnulib module mempcpy ## begin gnulib module msvc-inval EXTRA_DIST += msvc-inval.c msvc-inval.h EXTRA_libgnu_la_SOURCES += msvc-inval.c ## end gnulib module msvc-inval ## begin gnulib module msvc-nothrow EXTRA_DIST += msvc-nothrow.c msvc-nothrow.h EXTRA_libgnu_la_SOURCES += msvc-nothrow.c ## end gnulib module msvc-nothrow ## begin gnulib module nl_langinfo EXTRA_DIST += nl_langinfo.c EXTRA_libgnu_la_SOURCES += nl_langinfo.c ## end gnulib module nl_langinfo ## begin gnulib module nproc libgnu_la_SOURCES += nproc.c EXTRA_DIST += nproc.h ## end gnulib module nproc ## begin gnulib module rawmemchr EXTRA_DIST += rawmemchr.c rawmemchr.valgrind EXTRA_libgnu_la_SOURCES += rawmemchr.c ## end gnulib module rawmemchr ## begin gnulib module regex EXTRA_DIST += regcomp.c regex.c regex.h regex_internal.c regex_internal.h regexec.c EXTRA_libgnu_la_SOURCES += regcomp.c regex.c regex_internal.c regexec.c ## end gnulib module regex ## begin gnulib module size_max libgnu_la_SOURCES += size_max.h ## end gnulib module size_max ## begin gnulib module sleep EXTRA_DIST += sleep.c EXTRA_libgnu_la_SOURCES += sleep.c ## end gnulib module sleep ## begin gnulib module snippet/_Noreturn # Because this Makefile snippet defines a variable used by other # gnulib Makefile snippets, it must be present in all Makefile.am that # need it. This is ensured by the applicability 'all' defined above. _NORETURN_H=$(top_srcdir)/bootstrapped/build-aux/snippet/_Noreturn.h EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/snippet/_Noreturn.h ## end gnulib module snippet/_Noreturn ## begin gnulib module snippet/arg-nonnull # The BUILT_SOURCES created by this Makefile snippet are not used via #include # statements but through direct file reference. Therefore this snippet must be # present in all Makefile.am that need it. This is ensured by the applicability # 'all' defined above. BUILT_SOURCES += arg-nonnull.h # The arg-nonnull.h that gets inserted into generated .h files is the same as # build-aux/snippet/arg-nonnull.h, except that it has the copyright header cut # off. arg-nonnull.h: $(top_srcdir)/bootstrapped/build-aux/snippet/arg-nonnull.h $(AM_V_GEN)rm -f $@-t $@ && \ sed -n -e '/GL_ARG_NONNULL/,$$p' \ < $(top_srcdir)/bootstrapped/build-aux/snippet/arg-nonnull.h \ > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += arg-nonnull.h arg-nonnull.h-t ARG_NONNULL_H=arg-nonnull.h EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/snippet/arg-nonnull.h ## end gnulib module snippet/arg-nonnull ## begin gnulib module snippet/c++defs # The BUILT_SOURCES created by this Makefile snippet are not used via #include # statements but through direct file reference. Therefore this snippet must be # present in all Makefile.am that need it. This is ensured by the applicability # 'all' defined above. BUILT_SOURCES += c++defs.h # The c++defs.h that gets inserted into generated .h files is the same as # build-aux/snippet/c++defs.h, except that it has the copyright header cut off. c++defs.h: $(top_srcdir)/bootstrapped/build-aux/snippet/c++defs.h $(AM_V_GEN)rm -f $@-t $@ && \ sed -n -e '/_GL_CXXDEFS/,$$p' \ < $(top_srcdir)/bootstrapped/build-aux/snippet/c++defs.h \ > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += c++defs.h c++defs.h-t CXXDEFS_H=c++defs.h EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/snippet/c++defs.h ## end gnulib module snippet/c++defs ## begin gnulib module snippet/warn-on-use BUILT_SOURCES += warn-on-use.h # The warn-on-use.h that gets inserted into generated .h files is the same as # build-aux/snippet/warn-on-use.h, except that it has the copyright header cut # off. warn-on-use.h: $(top_srcdir)/bootstrapped/build-aux/snippet/warn-on-use.h $(AM_V_GEN)rm -f $@-t $@ && \ sed -n -e '/^.ifndef/,$$p' \ < $(top_srcdir)/bootstrapped/build-aux/snippet/warn-on-use.h \ > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += warn-on-use.h warn-on-use.h-t WARN_ON_USE_H=warn-on-use.h EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/snippet/warn-on-use.h ## end gnulib module snippet/warn-on-use ## begin gnulib module stdalign BUILT_SOURCES += $(STDALIGN_H) # We need the following in order to create when the system # doesn't have one that works. if GL_GENERATE_STDALIGN_H stdalign.h: stdalign.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ cat $(srcdir)/stdalign.in.h; \ } > $@-t && \ mv $@-t $@ else stdalign.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += stdalign.h stdalign.h-t EXTRA_DIST += stdalign.in.h ## end gnulib module stdalign ## begin gnulib module stdbool BUILT_SOURCES += $(STDBOOL_H) # We need the following in order to create when the system # doesn't have one that works. if GL_GENERATE_STDBOOL_H stdbool.h: stdbool.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's/@''HAVE__BOOL''@/$(HAVE__BOOL)/g' < $(srcdir)/stdbool.in.h; \ } > $@-t && \ mv $@-t $@ else stdbool.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += stdbool.h stdbool.h-t EXTRA_DIST += stdbool.in.h ## end gnulib module stdbool ## begin gnulib module stddef BUILT_SOURCES += $(STDDEF_H) # We need the following in order to create when the system # doesn't have one that works with the given compiler. if GL_GENERATE_STDDEF_H stddef.h: stddef.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STDDEF_H''@|$(NEXT_STDDEF_H)|g' \ -e 's|@''HAVE_MAX_ALIGN_T''@|$(HAVE_MAX_ALIGN_T)|g' \ -e 's|@''HAVE_WCHAR_T''@|$(HAVE_WCHAR_T)|g' \ -e 's|@''REPLACE_NULL''@|$(REPLACE_NULL)|g' \ < $(srcdir)/stddef.in.h; \ } > $@-t && \ mv $@-t $@ else stddef.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += stddef.h stddef.h-t EXTRA_DIST += stddef.in.h ## end gnulib module stddef ## begin gnulib module stdint BUILT_SOURCES += $(STDINT_H) # We need the following in order to create when the system # doesn't have one that works with the given compiler. if GL_GENERATE_STDINT_H stdint.h: stdint.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's/@''HAVE_STDINT_H''@/$(HAVE_STDINT_H)/g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STDINT_H''@|$(NEXT_STDINT_H)|g' \ -e 's/@''HAVE_C99_STDINT_H''@/$(HAVE_C99_STDINT_H)/g' \ -e 's/@''HAVE_SYS_TYPES_H''@/$(HAVE_SYS_TYPES_H)/g' \ -e 's/@''HAVE_INTTYPES_H''@/$(HAVE_INTTYPES_H)/g' \ -e 's/@''HAVE_SYS_INTTYPES_H''@/$(HAVE_SYS_INTTYPES_H)/g' \ -e 's/@''HAVE_SYS_BITYPES_H''@/$(HAVE_SYS_BITYPES_H)/g' \ -e 's/@''HAVE_WCHAR_H''@/$(HAVE_WCHAR_H)/g' \ -e 's/@''HAVE_LONG_LONG_INT''@/$(HAVE_LONG_LONG_INT)/g' \ -e 's/@''HAVE_UNSIGNED_LONG_LONG_INT''@/$(HAVE_UNSIGNED_LONG_LONG_INT)/g' \ -e 's/@''APPLE_UNIVERSAL_BUILD''@/$(APPLE_UNIVERSAL_BUILD)/g' \ -e 's/@''BITSIZEOF_PTRDIFF_T''@/$(BITSIZEOF_PTRDIFF_T)/g' \ -e 's/@''PTRDIFF_T_SUFFIX''@/$(PTRDIFF_T_SUFFIX)/g' \ -e 's/@''BITSIZEOF_SIG_ATOMIC_T''@/$(BITSIZEOF_SIG_ATOMIC_T)/g' \ -e 's/@''HAVE_SIGNED_SIG_ATOMIC_T''@/$(HAVE_SIGNED_SIG_ATOMIC_T)/g' \ -e 's/@''SIG_ATOMIC_T_SUFFIX''@/$(SIG_ATOMIC_T_SUFFIX)/g' \ -e 's/@''BITSIZEOF_SIZE_T''@/$(BITSIZEOF_SIZE_T)/g' \ -e 's/@''SIZE_T_SUFFIX''@/$(SIZE_T_SUFFIX)/g' \ -e 's/@''BITSIZEOF_WCHAR_T''@/$(BITSIZEOF_WCHAR_T)/g' \ -e 's/@''HAVE_SIGNED_WCHAR_T''@/$(HAVE_SIGNED_WCHAR_T)/g' \ -e 's/@''WCHAR_T_SUFFIX''@/$(WCHAR_T_SUFFIX)/g' \ -e 's/@''BITSIZEOF_WINT_T''@/$(BITSIZEOF_WINT_T)/g' \ -e 's/@''HAVE_SIGNED_WINT_T''@/$(HAVE_SIGNED_WINT_T)/g' \ -e 's/@''WINT_T_SUFFIX''@/$(WINT_T_SUFFIX)/g' \ < $(srcdir)/stdint.in.h; \ } > $@-t && \ mv $@-t $@ else stdint.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += stdint.h stdint.h-t EXTRA_DIST += stdint.in.h ## end gnulib module stdint ## begin gnulib module stdio BUILT_SOURCES += stdio.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. stdio.h: stdio.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STDIO_H''@|$(NEXT_STDIO_H)|g' \ -e 's/@''GNULIB_DPRINTF''@/$(GNULIB_DPRINTF)/g' \ -e 's/@''GNULIB_FCLOSE''@/$(GNULIB_FCLOSE)/g' \ -e 's/@''GNULIB_FDOPEN''@/$(GNULIB_FDOPEN)/g' \ -e 's/@''GNULIB_FFLUSH''@/$(GNULIB_FFLUSH)/g' \ -e 's/@''GNULIB_FGETC''@/$(GNULIB_FGETC)/g' \ -e 's/@''GNULIB_FGETS''@/$(GNULIB_FGETS)/g' \ -e 's/@''GNULIB_FOPEN''@/$(GNULIB_FOPEN)/g' \ -e 's/@''GNULIB_FPRINTF''@/$(GNULIB_FPRINTF)/g' \ -e 's/@''GNULIB_FPRINTF_POSIX''@/$(GNULIB_FPRINTF_POSIX)/g' \ -e 's/@''GNULIB_FPURGE''@/$(GNULIB_FPURGE)/g' \ -e 's/@''GNULIB_FPUTC''@/$(GNULIB_FPUTC)/g' \ -e 's/@''GNULIB_FPUTS''@/$(GNULIB_FPUTS)/g' \ -e 's/@''GNULIB_FREAD''@/$(GNULIB_FREAD)/g' \ -e 's/@''GNULIB_FREOPEN''@/$(GNULIB_FREOPEN)/g' \ -e 's/@''GNULIB_FSCANF''@/$(GNULIB_FSCANF)/g' \ -e 's/@''GNULIB_FSEEK''@/$(GNULIB_FSEEK)/g' \ -e 's/@''GNULIB_FSEEKO''@/$(GNULIB_FSEEKO)/g' \ -e 's/@''GNULIB_FTELL''@/$(GNULIB_FTELL)/g' \ -e 's/@''GNULIB_FTELLO''@/$(GNULIB_FTELLO)/g' \ -e 's/@''GNULIB_FWRITE''@/$(GNULIB_FWRITE)/g' \ -e 's/@''GNULIB_GETC''@/$(GNULIB_GETC)/g' \ -e 's/@''GNULIB_GETCHAR''@/$(GNULIB_GETCHAR)/g' \ -e 's/@''GNULIB_GETDELIM''@/$(GNULIB_GETDELIM)/g' \ -e 's/@''GNULIB_GETLINE''@/$(GNULIB_GETLINE)/g' \ -e 's/@''GNULIB_OBSTACK_PRINTF''@/$(GNULIB_OBSTACK_PRINTF)/g' \ -e 's/@''GNULIB_OBSTACK_PRINTF_POSIX''@/$(GNULIB_OBSTACK_PRINTF_POSIX)/g' \ -e 's/@''GNULIB_PCLOSE''@/$(GNULIB_PCLOSE)/g' \ -e 's/@''GNULIB_PERROR''@/$(GNULIB_PERROR)/g' \ -e 's/@''GNULIB_POPEN''@/$(GNULIB_POPEN)/g' \ -e 's/@''GNULIB_PRINTF''@/$(GNULIB_PRINTF)/g' \ -e 's/@''GNULIB_PRINTF_POSIX''@/$(GNULIB_PRINTF_POSIX)/g' \ -e 's/@''GNULIB_PUTC''@/$(GNULIB_PUTC)/g' \ -e 's/@''GNULIB_PUTCHAR''@/$(GNULIB_PUTCHAR)/g' \ -e 's/@''GNULIB_PUTS''@/$(GNULIB_PUTS)/g' \ -e 's/@''GNULIB_REMOVE''@/$(GNULIB_REMOVE)/g' \ -e 's/@''GNULIB_RENAME''@/$(GNULIB_RENAME)/g' \ -e 's/@''GNULIB_RENAMEAT''@/$(GNULIB_RENAMEAT)/g' \ -e 's/@''GNULIB_SCANF''@/$(GNULIB_SCANF)/g' \ -e 's/@''GNULIB_SNPRINTF''@/$(GNULIB_SNPRINTF)/g' \ -e 's/@''GNULIB_SPRINTF_POSIX''@/$(GNULIB_SPRINTF_POSIX)/g' \ -e 's/@''GNULIB_STDIO_H_NONBLOCKING''@/$(GNULIB_STDIO_H_NONBLOCKING)/g' \ -e 's/@''GNULIB_STDIO_H_SIGPIPE''@/$(GNULIB_STDIO_H_SIGPIPE)/g' \ -e 's/@''GNULIB_TMPFILE''@/$(GNULIB_TMPFILE)/g' \ -e 's/@''GNULIB_VASPRINTF''@/$(GNULIB_VASPRINTF)/g' \ -e 's/@''GNULIB_VDPRINTF''@/$(GNULIB_VDPRINTF)/g' \ -e 's/@''GNULIB_VFPRINTF''@/$(GNULIB_VFPRINTF)/g' \ -e 's/@''GNULIB_VFPRINTF_POSIX''@/$(GNULIB_VFPRINTF_POSIX)/g' \ -e 's/@''GNULIB_VFSCANF''@/$(GNULIB_VFSCANF)/g' \ -e 's/@''GNULIB_VSCANF''@/$(GNULIB_VSCANF)/g' \ -e 's/@''GNULIB_VPRINTF''@/$(GNULIB_VPRINTF)/g' \ -e 's/@''GNULIB_VPRINTF_POSIX''@/$(GNULIB_VPRINTF_POSIX)/g' \ -e 's/@''GNULIB_VSNPRINTF''@/$(GNULIB_VSNPRINTF)/g' \ -e 's/@''GNULIB_VSPRINTF_POSIX''@/$(GNULIB_VSPRINTF_POSIX)/g' \ < $(srcdir)/stdio.in.h | \ sed -e 's|@''HAVE_DECL_FPURGE''@|$(HAVE_DECL_FPURGE)|g' \ -e 's|@''HAVE_DECL_FSEEKO''@|$(HAVE_DECL_FSEEKO)|g' \ -e 's|@''HAVE_DECL_FTELLO''@|$(HAVE_DECL_FTELLO)|g' \ -e 's|@''HAVE_DECL_GETDELIM''@|$(HAVE_DECL_GETDELIM)|g' \ -e 's|@''HAVE_DECL_GETLINE''@|$(HAVE_DECL_GETLINE)|g' \ -e 's|@''HAVE_DECL_OBSTACK_PRINTF''@|$(HAVE_DECL_OBSTACK_PRINTF)|g' \ -e 's|@''HAVE_DECL_SNPRINTF''@|$(HAVE_DECL_SNPRINTF)|g' \ -e 's|@''HAVE_DECL_VSNPRINTF''@|$(HAVE_DECL_VSNPRINTF)|g' \ -e 's|@''HAVE_DPRINTF''@|$(HAVE_DPRINTF)|g' \ -e 's|@''HAVE_FSEEKO''@|$(HAVE_FSEEKO)|g' \ -e 's|@''HAVE_FTELLO''@|$(HAVE_FTELLO)|g' \ -e 's|@''HAVE_PCLOSE''@|$(HAVE_PCLOSE)|g' \ -e 's|@''HAVE_POPEN''@|$(HAVE_POPEN)|g' \ -e 's|@''HAVE_RENAMEAT''@|$(HAVE_RENAMEAT)|g' \ -e 's|@''HAVE_VASPRINTF''@|$(HAVE_VASPRINTF)|g' \ -e 's|@''HAVE_VDPRINTF''@|$(HAVE_VDPRINTF)|g' \ -e 's|@''REPLACE_DPRINTF''@|$(REPLACE_DPRINTF)|g' \ -e 's|@''REPLACE_FCLOSE''@|$(REPLACE_FCLOSE)|g' \ -e 's|@''REPLACE_FDOPEN''@|$(REPLACE_FDOPEN)|g' \ -e 's|@''REPLACE_FFLUSH''@|$(REPLACE_FFLUSH)|g' \ -e 's|@''REPLACE_FOPEN''@|$(REPLACE_FOPEN)|g' \ -e 's|@''REPLACE_FPRINTF''@|$(REPLACE_FPRINTF)|g' \ -e 's|@''REPLACE_FPURGE''@|$(REPLACE_FPURGE)|g' \ -e 's|@''REPLACE_FREOPEN''@|$(REPLACE_FREOPEN)|g' \ -e 's|@''REPLACE_FSEEK''@|$(REPLACE_FSEEK)|g' \ -e 's|@''REPLACE_FSEEKO''@|$(REPLACE_FSEEKO)|g' \ -e 's|@''REPLACE_FTELL''@|$(REPLACE_FTELL)|g' \ -e 's|@''REPLACE_FTELLO''@|$(REPLACE_FTELLO)|g' \ -e 's|@''REPLACE_GETDELIM''@|$(REPLACE_GETDELIM)|g' \ -e 's|@''REPLACE_GETLINE''@|$(REPLACE_GETLINE)|g' \ -e 's|@''REPLACE_OBSTACK_PRINTF''@|$(REPLACE_OBSTACK_PRINTF)|g' \ -e 's|@''REPLACE_PERROR''@|$(REPLACE_PERROR)|g' \ -e 's|@''REPLACE_POPEN''@|$(REPLACE_POPEN)|g' \ -e 's|@''REPLACE_PRINTF''@|$(REPLACE_PRINTF)|g' \ -e 's|@''REPLACE_REMOVE''@|$(REPLACE_REMOVE)|g' \ -e 's|@''REPLACE_RENAME''@|$(REPLACE_RENAME)|g' \ -e 's|@''REPLACE_RENAMEAT''@|$(REPLACE_RENAMEAT)|g' \ -e 's|@''REPLACE_SNPRINTF''@|$(REPLACE_SNPRINTF)|g' \ -e 's|@''REPLACE_SPRINTF''@|$(REPLACE_SPRINTF)|g' \ -e 's|@''REPLACE_STDIO_READ_FUNCS''@|$(REPLACE_STDIO_READ_FUNCS)|g' \ -e 's|@''REPLACE_STDIO_WRITE_FUNCS''@|$(REPLACE_STDIO_WRITE_FUNCS)|g' \ -e 's|@''REPLACE_TMPFILE''@|$(REPLACE_TMPFILE)|g' \ -e 's|@''REPLACE_VASPRINTF''@|$(REPLACE_VASPRINTF)|g' \ -e 's|@''REPLACE_VDPRINTF''@|$(REPLACE_VDPRINTF)|g' \ -e 's|@''REPLACE_VFPRINTF''@|$(REPLACE_VFPRINTF)|g' \ -e 's|@''REPLACE_VPRINTF''@|$(REPLACE_VPRINTF)|g' \ -e 's|@''REPLACE_VSNPRINTF''@|$(REPLACE_VSNPRINTF)|g' \ -e 's|@''REPLACE_VSPRINTF''@|$(REPLACE_VSPRINTF)|g' \ -e 's|@''ASM_SYMBOL_PREFIX''@|$(ASM_SYMBOL_PREFIX)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += stdio.h stdio.h-t EXTRA_DIST += stdio.in.h ## end gnulib module stdio ## begin gnulib module stdlib BUILT_SOURCES += stdlib.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. stdlib.h: stdlib.in.h $(top_builddir)/config.status $(CXXDEFS_H) \ $(_NORETURN_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STDLIB_H''@|$(NEXT_STDLIB_H)|g' \ -e 's/@''GNULIB__EXIT''@/$(GNULIB__EXIT)/g' \ -e 's/@''GNULIB_ATOLL''@/$(GNULIB_ATOLL)/g' \ -e 's/@''GNULIB_CALLOC_POSIX''@/$(GNULIB_CALLOC_POSIX)/g' \ -e 's/@''GNULIB_CANONICALIZE_FILE_NAME''@/$(GNULIB_CANONICALIZE_FILE_NAME)/g' \ -e 's/@''GNULIB_GETLOADAVG''@/$(GNULIB_GETLOADAVG)/g' \ -e 's/@''GNULIB_GETSUBOPT''@/$(GNULIB_GETSUBOPT)/g' \ -e 's/@''GNULIB_GRANTPT''@/$(GNULIB_GRANTPT)/g' \ -e 's/@''GNULIB_MALLOC_POSIX''@/$(GNULIB_MALLOC_POSIX)/g' \ -e 's/@''GNULIB_MBTOWC''@/$(GNULIB_MBTOWC)/g' \ -e 's/@''GNULIB_MKDTEMP''@/$(GNULIB_MKDTEMP)/g' \ -e 's/@''GNULIB_MKOSTEMP''@/$(GNULIB_MKOSTEMP)/g' \ -e 's/@''GNULIB_MKOSTEMPS''@/$(GNULIB_MKOSTEMPS)/g' \ -e 's/@''GNULIB_MKSTEMP''@/$(GNULIB_MKSTEMP)/g' \ -e 's/@''GNULIB_MKSTEMPS''@/$(GNULIB_MKSTEMPS)/g' \ -e 's/@''GNULIB_POSIX_OPENPT''@/$(GNULIB_POSIX_OPENPT)/g' \ -e 's/@''GNULIB_PTSNAME''@/$(GNULIB_PTSNAME)/g' \ -e 's/@''GNULIB_PTSNAME_R''@/$(GNULIB_PTSNAME_R)/g' \ -e 's/@''GNULIB_PUTENV''@/$(GNULIB_PUTENV)/g' \ -e 's/@''GNULIB_QSORT_R''@/$(GNULIB_QSORT_R)/g' \ -e 's/@''GNULIB_RANDOM''@/$(GNULIB_RANDOM)/g' \ -e 's/@''GNULIB_RANDOM_R''@/$(GNULIB_RANDOM_R)/g' \ -e 's/@''GNULIB_REALLOC_POSIX''@/$(GNULIB_REALLOC_POSIX)/g' \ -e 's/@''GNULIB_REALPATH''@/$(GNULIB_REALPATH)/g' \ -e 's/@''GNULIB_RPMATCH''@/$(GNULIB_RPMATCH)/g' \ -e 's/@''GNULIB_SECURE_GETENV''@/$(GNULIB_SECURE_GETENV)/g' \ -e 's/@''GNULIB_SETENV''@/$(GNULIB_SETENV)/g' \ -e 's/@''GNULIB_STRTOD''@/$(GNULIB_STRTOD)/g' \ -e 's/@''GNULIB_STRTOLL''@/$(GNULIB_STRTOLL)/g' \ -e 's/@''GNULIB_STRTOULL''@/$(GNULIB_STRTOULL)/g' \ -e 's/@''GNULIB_SYSTEM_POSIX''@/$(GNULIB_SYSTEM_POSIX)/g' \ -e 's/@''GNULIB_UNLOCKPT''@/$(GNULIB_UNLOCKPT)/g' \ -e 's/@''GNULIB_UNSETENV''@/$(GNULIB_UNSETENV)/g' \ -e 's/@''GNULIB_WCTOMB''@/$(GNULIB_WCTOMB)/g' \ < $(srcdir)/stdlib.in.h | \ sed -e 's|@''HAVE__EXIT''@|$(HAVE__EXIT)|g' \ -e 's|@''HAVE_ATOLL''@|$(HAVE_ATOLL)|g' \ -e 's|@''HAVE_CANONICALIZE_FILE_NAME''@|$(HAVE_CANONICALIZE_FILE_NAME)|g' \ -e 's|@''HAVE_DECL_GETLOADAVG''@|$(HAVE_DECL_GETLOADAVG)|g' \ -e 's|@''HAVE_GETSUBOPT''@|$(HAVE_GETSUBOPT)|g' \ -e 's|@''HAVE_GRANTPT''@|$(HAVE_GRANTPT)|g' \ -e 's|@''HAVE_MKDTEMP''@|$(HAVE_MKDTEMP)|g' \ -e 's|@''HAVE_MKOSTEMP''@|$(HAVE_MKOSTEMP)|g' \ -e 's|@''HAVE_MKOSTEMPS''@|$(HAVE_MKOSTEMPS)|g' \ -e 's|@''HAVE_MKSTEMP''@|$(HAVE_MKSTEMP)|g' \ -e 's|@''HAVE_MKSTEMPS''@|$(HAVE_MKSTEMPS)|g' \ -e 's|@''HAVE_POSIX_OPENPT''@|$(HAVE_POSIX_OPENPT)|g' \ -e 's|@''HAVE_PTSNAME''@|$(HAVE_PTSNAME)|g' \ -e 's|@''HAVE_PTSNAME_R''@|$(HAVE_PTSNAME_R)|g' \ -e 's|@''HAVE_QSORT_R''@|$(HAVE_QSORT_R)|g' \ -e 's|@''HAVE_RANDOM''@|$(HAVE_RANDOM)|g' \ -e 's|@''HAVE_RANDOM_H''@|$(HAVE_RANDOM_H)|g' \ -e 's|@''HAVE_RANDOM_R''@|$(HAVE_RANDOM_R)|g' \ -e 's|@''HAVE_REALPATH''@|$(HAVE_REALPATH)|g' \ -e 's|@''HAVE_RPMATCH''@|$(HAVE_RPMATCH)|g' \ -e 's|@''HAVE_SECURE_GETENV''@|$(HAVE_SECURE_GETENV)|g' \ -e 's|@''HAVE_DECL_SETENV''@|$(HAVE_DECL_SETENV)|g' \ -e 's|@''HAVE_STRTOD''@|$(HAVE_STRTOD)|g' \ -e 's|@''HAVE_STRTOLL''@|$(HAVE_STRTOLL)|g' \ -e 's|@''HAVE_STRTOULL''@|$(HAVE_STRTOULL)|g' \ -e 's|@''HAVE_STRUCT_RANDOM_DATA''@|$(HAVE_STRUCT_RANDOM_DATA)|g' \ -e 's|@''HAVE_SYS_LOADAVG_H''@|$(HAVE_SYS_LOADAVG_H)|g' \ -e 's|@''HAVE_UNLOCKPT''@|$(HAVE_UNLOCKPT)|g' \ -e 's|@''HAVE_DECL_UNSETENV''@|$(HAVE_DECL_UNSETENV)|g' \ -e 's|@''REPLACE_CALLOC''@|$(REPLACE_CALLOC)|g' \ -e 's|@''REPLACE_CANONICALIZE_FILE_NAME''@|$(REPLACE_CANONICALIZE_FILE_NAME)|g' \ -e 's|@''REPLACE_MALLOC''@|$(REPLACE_MALLOC)|g' \ -e 's|@''REPLACE_MBTOWC''@|$(REPLACE_MBTOWC)|g' \ -e 's|@''REPLACE_MKSTEMP''@|$(REPLACE_MKSTEMP)|g' \ -e 's|@''REPLACE_PTSNAME''@|$(REPLACE_PTSNAME)|g' \ -e 's|@''REPLACE_PTSNAME_R''@|$(REPLACE_PTSNAME_R)|g' \ -e 's|@''REPLACE_PUTENV''@|$(REPLACE_PUTENV)|g' \ -e 's|@''REPLACE_QSORT_R''@|$(REPLACE_QSORT_R)|g' \ -e 's|@''REPLACE_RANDOM_R''@|$(REPLACE_RANDOM_R)|g' \ -e 's|@''REPLACE_REALLOC''@|$(REPLACE_REALLOC)|g' \ -e 's|@''REPLACE_REALPATH''@|$(REPLACE_REALPATH)|g' \ -e 's|@''REPLACE_SETENV''@|$(REPLACE_SETENV)|g' \ -e 's|@''REPLACE_STRTOD''@|$(REPLACE_STRTOD)|g' \ -e 's|@''REPLACE_UNSETENV''@|$(REPLACE_UNSETENV)|g' \ -e 's|@''REPLACE_WCTOMB''@|$(REPLACE_WCTOMB)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _Noreturn/r $(_NORETURN_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += stdlib.h stdlib.h-t EXTRA_DIST += stdlib.in.h ## end gnulib module stdlib ## begin gnulib module strcase EXTRA_DIST += strcasecmp.c strncasecmp.c EXTRA_libgnu_la_SOURCES += strcasecmp.c strncasecmp.c ## end gnulib module strcase ## begin gnulib module strchrnul EXTRA_DIST += strchrnul.c strchrnul.valgrind EXTRA_libgnu_la_SOURCES += strchrnul.c ## end gnulib module strchrnul ## begin gnulib module streq EXTRA_DIST += streq.h ## end gnulib module streq ## begin gnulib module strerror EXTRA_DIST += strerror.c EXTRA_libgnu_la_SOURCES += strerror.c ## end gnulib module strerror ## begin gnulib module strerror-override EXTRA_DIST += strerror-override.c strerror-override.h EXTRA_libgnu_la_SOURCES += strerror-override.c ## end gnulib module strerror-override ## begin gnulib module string BUILT_SOURCES += string.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. string.h: string.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STRING_H''@|$(NEXT_STRING_H)|g' \ -e 's/@''GNULIB_FFSL''@/$(GNULIB_FFSL)/g' \ -e 's/@''GNULIB_FFSLL''@/$(GNULIB_FFSLL)/g' \ -e 's/@''GNULIB_MBSLEN''@/$(GNULIB_MBSLEN)/g' \ -e 's/@''GNULIB_MBSNLEN''@/$(GNULIB_MBSNLEN)/g' \ -e 's/@''GNULIB_MBSCHR''@/$(GNULIB_MBSCHR)/g' \ -e 's/@''GNULIB_MBSRCHR''@/$(GNULIB_MBSRCHR)/g' \ -e 's/@''GNULIB_MBSSTR''@/$(GNULIB_MBSSTR)/g' \ -e 's/@''GNULIB_MBSCASECMP''@/$(GNULIB_MBSCASECMP)/g' \ -e 's/@''GNULIB_MBSNCASECMP''@/$(GNULIB_MBSNCASECMP)/g' \ -e 's/@''GNULIB_MBSPCASECMP''@/$(GNULIB_MBSPCASECMP)/g' \ -e 's/@''GNULIB_MBSCASESTR''@/$(GNULIB_MBSCASESTR)/g' \ -e 's/@''GNULIB_MBSCSPN''@/$(GNULIB_MBSCSPN)/g' \ -e 's/@''GNULIB_MBSPBRK''@/$(GNULIB_MBSPBRK)/g' \ -e 's/@''GNULIB_MBSSPN''@/$(GNULIB_MBSSPN)/g' \ -e 's/@''GNULIB_MBSSEP''@/$(GNULIB_MBSSEP)/g' \ -e 's/@''GNULIB_MBSTOK_R''@/$(GNULIB_MBSTOK_R)/g' \ -e 's/@''GNULIB_MEMCHR''@/$(GNULIB_MEMCHR)/g' \ -e 's/@''GNULIB_MEMMEM''@/$(GNULIB_MEMMEM)/g' \ -e 's/@''GNULIB_MEMPCPY''@/$(GNULIB_MEMPCPY)/g' \ -e 's/@''GNULIB_MEMRCHR''@/$(GNULIB_MEMRCHR)/g' \ -e 's/@''GNULIB_RAWMEMCHR''@/$(GNULIB_RAWMEMCHR)/g' \ -e 's/@''GNULIB_STPCPY''@/$(GNULIB_STPCPY)/g' \ -e 's/@''GNULIB_STPNCPY''@/$(GNULIB_STPNCPY)/g' \ -e 's/@''GNULIB_STRCHRNUL''@/$(GNULIB_STRCHRNUL)/g' \ -e 's/@''GNULIB_STRDUP''@/$(GNULIB_STRDUP)/g' \ -e 's/@''GNULIB_STRNCAT''@/$(GNULIB_STRNCAT)/g' \ -e 's/@''GNULIB_STRNDUP''@/$(GNULIB_STRNDUP)/g' \ -e 's/@''GNULIB_STRNLEN''@/$(GNULIB_STRNLEN)/g' \ -e 's/@''GNULIB_STRPBRK''@/$(GNULIB_STRPBRK)/g' \ -e 's/@''GNULIB_STRSEP''@/$(GNULIB_STRSEP)/g' \ -e 's/@''GNULIB_STRSTR''@/$(GNULIB_STRSTR)/g' \ -e 's/@''GNULIB_STRCASESTR''@/$(GNULIB_STRCASESTR)/g' \ -e 's/@''GNULIB_STRTOK_R''@/$(GNULIB_STRTOK_R)/g' \ -e 's/@''GNULIB_STRERROR''@/$(GNULIB_STRERROR)/g' \ -e 's/@''GNULIB_STRERROR_R''@/$(GNULIB_STRERROR_R)/g' \ -e 's/@''GNULIB_STRSIGNAL''@/$(GNULIB_STRSIGNAL)/g' \ -e 's/@''GNULIB_STRVERSCMP''@/$(GNULIB_STRVERSCMP)/g' \ < $(srcdir)/string.in.h | \ sed -e 's|@''HAVE_FFSL''@|$(HAVE_FFSL)|g' \ -e 's|@''HAVE_FFSLL''@|$(HAVE_FFSLL)|g' \ -e 's|@''HAVE_MBSLEN''@|$(HAVE_MBSLEN)|g' \ -e 's|@''HAVE_MEMCHR''@|$(HAVE_MEMCHR)|g' \ -e 's|@''HAVE_DECL_MEMMEM''@|$(HAVE_DECL_MEMMEM)|g' \ -e 's|@''HAVE_MEMPCPY''@|$(HAVE_MEMPCPY)|g' \ -e 's|@''HAVE_DECL_MEMRCHR''@|$(HAVE_DECL_MEMRCHR)|g' \ -e 's|@''HAVE_RAWMEMCHR''@|$(HAVE_RAWMEMCHR)|g' \ -e 's|@''HAVE_STPCPY''@|$(HAVE_STPCPY)|g' \ -e 's|@''HAVE_STPNCPY''@|$(HAVE_STPNCPY)|g' \ -e 's|@''HAVE_STRCHRNUL''@|$(HAVE_STRCHRNUL)|g' \ -e 's|@''HAVE_DECL_STRDUP''@|$(HAVE_DECL_STRDUP)|g' \ -e 's|@''HAVE_DECL_STRNDUP''@|$(HAVE_DECL_STRNDUP)|g' \ -e 's|@''HAVE_DECL_STRNLEN''@|$(HAVE_DECL_STRNLEN)|g' \ -e 's|@''HAVE_STRPBRK''@|$(HAVE_STRPBRK)|g' \ -e 's|@''HAVE_STRSEP''@|$(HAVE_STRSEP)|g' \ -e 's|@''HAVE_STRCASESTR''@|$(HAVE_STRCASESTR)|g' \ -e 's|@''HAVE_DECL_STRTOK_R''@|$(HAVE_DECL_STRTOK_R)|g' \ -e 's|@''HAVE_DECL_STRERROR_R''@|$(HAVE_DECL_STRERROR_R)|g' \ -e 's|@''HAVE_DECL_STRSIGNAL''@|$(HAVE_DECL_STRSIGNAL)|g' \ -e 's|@''HAVE_STRVERSCMP''@|$(HAVE_STRVERSCMP)|g' \ -e 's|@''REPLACE_STPNCPY''@|$(REPLACE_STPNCPY)|g' \ -e 's|@''REPLACE_MEMCHR''@|$(REPLACE_MEMCHR)|g' \ -e 's|@''REPLACE_MEMMEM''@|$(REPLACE_MEMMEM)|g' \ -e 's|@''REPLACE_STRCASESTR''@|$(REPLACE_STRCASESTR)|g' \ -e 's|@''REPLACE_STRCHRNUL''@|$(REPLACE_STRCHRNUL)|g' \ -e 's|@''REPLACE_STRDUP''@|$(REPLACE_STRDUP)|g' \ -e 's|@''REPLACE_STRSTR''@|$(REPLACE_STRSTR)|g' \ -e 's|@''REPLACE_STRERROR''@|$(REPLACE_STRERROR)|g' \ -e 's|@''REPLACE_STRERROR_R''@|$(REPLACE_STRERROR_R)|g' \ -e 's|@''REPLACE_STRNCAT''@|$(REPLACE_STRNCAT)|g' \ -e 's|@''REPLACE_STRNDUP''@|$(REPLACE_STRNDUP)|g' \ -e 's|@''REPLACE_STRNLEN''@|$(REPLACE_STRNLEN)|g' \ -e 's|@''REPLACE_STRSIGNAL''@|$(REPLACE_STRSIGNAL)|g' \ -e 's|@''REPLACE_STRTOK_R''@|$(REPLACE_STRTOK_R)|g' \ -e 's|@''UNDEFINE_STRTOK_R''@|$(UNDEFINE_STRTOK_R)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ < $(srcdir)/string.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += string.h string.h-t EXTRA_DIST += string.in.h ## end gnulib module string ## begin gnulib module strings BUILT_SOURCES += strings.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. strings.h: strings.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(ARG_NONNULL_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''HAVE_STRINGS_H''@|$(HAVE_STRINGS_H)|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STRINGS_H''@|$(NEXT_STRINGS_H)|g' \ -e 's|@''GNULIB_FFS''@|$(GNULIB_FFS)|g' \ -e 's|@''HAVE_FFS''@|$(HAVE_FFS)|g' \ -e 's|@''HAVE_STRCASECMP''@|$(HAVE_STRCASECMP)|g' \ -e 's|@''HAVE_DECL_STRNCASECMP''@|$(HAVE_DECL_STRNCASECMP)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/strings.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += strings.h strings.h-t EXTRA_DIST += strings.in.h ## end gnulib module strings ## begin gnulib module strndup EXTRA_DIST += strndup.c EXTRA_libgnu_la_SOURCES += strndup.c ## end gnulib module strndup ## begin gnulib module strnlen EXTRA_DIST += strnlen.c EXTRA_libgnu_la_SOURCES += strnlen.c ## end gnulib module strnlen ## begin gnulib module sys_types BUILT_SOURCES += sys/types.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. sys/types.h: sys_types.in.h $(top_builddir)/config.status $(AM_V_at)$(MKDIR_P) sys $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_SYS_TYPES_H''@|$(NEXT_SYS_TYPES_H)|g' \ -e 's|@''WINDOWS_64_BIT_OFF_T''@|$(WINDOWS_64_BIT_OFF_T)|g' \ < $(srcdir)/sys_types.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += sys/types.h sys/types.h-t EXTRA_DIST += sys_types.in.h ## end gnulib module sys_types ## begin gnulib module sysexits BUILT_SOURCES += $(SYSEXITS_H) # We need the following in order to create when the system # doesn't have one that works with the given compiler. if GL_GENERATE_SYSEXITS_H sysexits.h: sysexits.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''HAVE_SYSEXITS_H''@|$(HAVE_SYSEXITS_H)|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_SYSEXITS_H''@|$(NEXT_SYSEXITS_H)|g' \ < $(srcdir)/sysexits.in.h; \ } > $@-t && \ mv -f $@-t $@ else sysexits.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += sysexits.h sysexits.h-t EXTRA_DIST += sysexits.in.h ## end gnulib module sysexits ## begin gnulib module threadlib libgnu_la_SOURCES += glthread/threadlib.c EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/config.rpath ## end gnulib module threadlib ## begin gnulib module unistd BUILT_SOURCES += unistd.h libgnu_la_SOURCES += unistd.c # We need the following in order to create an empty placeholder for # when the system doesn't have one. unistd.h: unistd.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''HAVE_UNISTD_H''@|$(HAVE_UNISTD_H)|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_UNISTD_H''@|$(NEXT_UNISTD_H)|g' \ -e 's|@''WINDOWS_64_BIT_OFF_T''@|$(WINDOWS_64_BIT_OFF_T)|g' \ -e 's/@''GNULIB_CHDIR''@/$(GNULIB_CHDIR)/g' \ -e 's/@''GNULIB_CHOWN''@/$(GNULIB_CHOWN)/g' \ -e 's/@''GNULIB_CLOSE''@/$(GNULIB_CLOSE)/g' \ -e 's/@''GNULIB_DUP''@/$(GNULIB_DUP)/g' \ -e 's/@''GNULIB_DUP2''@/$(GNULIB_DUP2)/g' \ -e 's/@''GNULIB_DUP3''@/$(GNULIB_DUP3)/g' \ -e 's/@''GNULIB_ENVIRON''@/$(GNULIB_ENVIRON)/g' \ -e 's/@''GNULIB_EUIDACCESS''@/$(GNULIB_EUIDACCESS)/g' \ -e 's/@''GNULIB_FACCESSAT''@/$(GNULIB_FACCESSAT)/g' \ -e 's/@''GNULIB_FCHDIR''@/$(GNULIB_FCHDIR)/g' \ -e 's/@''GNULIB_FCHOWNAT''@/$(GNULIB_FCHOWNAT)/g' \ -e 's/@''GNULIB_FDATASYNC''@/$(GNULIB_FDATASYNC)/g' \ -e 's/@''GNULIB_FSYNC''@/$(GNULIB_FSYNC)/g' \ -e 's/@''GNULIB_FTRUNCATE''@/$(GNULIB_FTRUNCATE)/g' \ -e 's/@''GNULIB_GETCWD''@/$(GNULIB_GETCWD)/g' \ -e 's/@''GNULIB_GETDOMAINNAME''@/$(GNULIB_GETDOMAINNAME)/g' \ -e 's/@''GNULIB_GETDTABLESIZE''@/$(GNULIB_GETDTABLESIZE)/g' \ -e 's/@''GNULIB_GETGROUPS''@/$(GNULIB_GETGROUPS)/g' \ -e 's/@''GNULIB_GETHOSTNAME''@/$(GNULIB_GETHOSTNAME)/g' \ -e 's/@''GNULIB_GETLOGIN''@/$(GNULIB_GETLOGIN)/g' \ -e 's/@''GNULIB_GETLOGIN_R''@/$(GNULIB_GETLOGIN_R)/g' \ -e 's/@''GNULIB_GETPAGESIZE''@/$(GNULIB_GETPAGESIZE)/g' \ -e 's/@''GNULIB_GETUSERSHELL''@/$(GNULIB_GETUSERSHELL)/g' \ -e 's/@''GNULIB_GROUP_MEMBER''@/$(GNULIB_GROUP_MEMBER)/g' \ -e 's/@''GNULIB_ISATTY''@/$(GNULIB_ISATTY)/g' \ -e 's/@''GNULIB_LCHOWN''@/$(GNULIB_LCHOWN)/g' \ -e 's/@''GNULIB_LINK''@/$(GNULIB_LINK)/g' \ -e 's/@''GNULIB_LINKAT''@/$(GNULIB_LINKAT)/g' \ -e 's/@''GNULIB_LSEEK''@/$(GNULIB_LSEEK)/g' \ -e 's/@''GNULIB_PIPE''@/$(GNULIB_PIPE)/g' \ -e 's/@''GNULIB_PIPE2''@/$(GNULIB_PIPE2)/g' \ -e 's/@''GNULIB_PREAD''@/$(GNULIB_PREAD)/g' \ -e 's/@''GNULIB_PWRITE''@/$(GNULIB_PWRITE)/g' \ -e 's/@''GNULIB_READ''@/$(GNULIB_READ)/g' \ -e 's/@''GNULIB_READLINK''@/$(GNULIB_READLINK)/g' \ -e 's/@''GNULIB_READLINKAT''@/$(GNULIB_READLINKAT)/g' \ -e 's/@''GNULIB_RMDIR''@/$(GNULIB_RMDIR)/g' \ -e 's/@''GNULIB_SETHOSTNAME''@/$(GNULIB_SETHOSTNAME)/g' \ -e 's/@''GNULIB_SLEEP''@/$(GNULIB_SLEEP)/g' \ -e 's/@''GNULIB_SYMLINK''@/$(GNULIB_SYMLINK)/g' \ -e 's/@''GNULIB_SYMLINKAT''@/$(GNULIB_SYMLINKAT)/g' \ -e 's/@''GNULIB_TTYNAME_R''@/$(GNULIB_TTYNAME_R)/g' \ -e 's/@''GNULIB_UNISTD_H_GETOPT''@/0$(GNULIB_GL_UNISTD_H_GETOPT)/g' \ -e 's/@''GNULIB_UNISTD_H_NONBLOCKING''@/$(GNULIB_UNISTD_H_NONBLOCKING)/g' \ -e 's/@''GNULIB_UNISTD_H_SIGPIPE''@/$(GNULIB_UNISTD_H_SIGPIPE)/g' \ -e 's/@''GNULIB_UNLINK''@/$(GNULIB_UNLINK)/g' \ -e 's/@''GNULIB_UNLINKAT''@/$(GNULIB_UNLINKAT)/g' \ -e 's/@''GNULIB_USLEEP''@/$(GNULIB_USLEEP)/g' \ -e 's/@''GNULIB_WRITE''@/$(GNULIB_WRITE)/g' \ < $(srcdir)/unistd.in.h | \ sed -e 's|@''HAVE_CHOWN''@|$(HAVE_CHOWN)|g' \ -e 's|@''HAVE_DUP2''@|$(HAVE_DUP2)|g' \ -e 's|@''HAVE_DUP3''@|$(HAVE_DUP3)|g' \ -e 's|@''HAVE_EUIDACCESS''@|$(HAVE_EUIDACCESS)|g' \ -e 's|@''HAVE_FACCESSAT''@|$(HAVE_FACCESSAT)|g' \ -e 's|@''HAVE_FCHDIR''@|$(HAVE_FCHDIR)|g' \ -e 's|@''HAVE_FCHOWNAT''@|$(HAVE_FCHOWNAT)|g' \ -e 's|@''HAVE_FDATASYNC''@|$(HAVE_FDATASYNC)|g' \ -e 's|@''HAVE_FSYNC''@|$(HAVE_FSYNC)|g' \ -e 's|@''HAVE_FTRUNCATE''@|$(HAVE_FTRUNCATE)|g' \ -e 's|@''HAVE_GETDTABLESIZE''@|$(HAVE_GETDTABLESIZE)|g' \ -e 's|@''HAVE_GETGROUPS''@|$(HAVE_GETGROUPS)|g' \ -e 's|@''HAVE_GETHOSTNAME''@|$(HAVE_GETHOSTNAME)|g' \ -e 's|@''HAVE_GETLOGIN''@|$(HAVE_GETLOGIN)|g' \ -e 's|@''HAVE_GETPAGESIZE''@|$(HAVE_GETPAGESIZE)|g' \ -e 's|@''HAVE_GROUP_MEMBER''@|$(HAVE_GROUP_MEMBER)|g' \ -e 's|@''HAVE_LCHOWN''@|$(HAVE_LCHOWN)|g' \ -e 's|@''HAVE_LINK''@|$(HAVE_LINK)|g' \ -e 's|@''HAVE_LINKAT''@|$(HAVE_LINKAT)|g' \ -e 's|@''HAVE_PIPE''@|$(HAVE_PIPE)|g' \ -e 's|@''HAVE_PIPE2''@|$(HAVE_PIPE2)|g' \ -e 's|@''HAVE_PREAD''@|$(HAVE_PREAD)|g' \ -e 's|@''HAVE_PWRITE''@|$(HAVE_PWRITE)|g' \ -e 's|@''HAVE_READLINK''@|$(HAVE_READLINK)|g' \ -e 's|@''HAVE_READLINKAT''@|$(HAVE_READLINKAT)|g' \ -e 's|@''HAVE_SETHOSTNAME''@|$(HAVE_SETHOSTNAME)|g' \ -e 's|@''HAVE_SLEEP''@|$(HAVE_SLEEP)|g' \ -e 's|@''HAVE_SYMLINK''@|$(HAVE_SYMLINK)|g' \ -e 's|@''HAVE_SYMLINKAT''@|$(HAVE_SYMLINKAT)|g' \ -e 's|@''HAVE_UNLINKAT''@|$(HAVE_UNLINKAT)|g' \ -e 's|@''HAVE_USLEEP''@|$(HAVE_USLEEP)|g' \ -e 's|@''HAVE_DECL_ENVIRON''@|$(HAVE_DECL_ENVIRON)|g' \ -e 's|@''HAVE_DECL_FCHDIR''@|$(HAVE_DECL_FCHDIR)|g' \ -e 's|@''HAVE_DECL_FDATASYNC''@|$(HAVE_DECL_FDATASYNC)|g' \ -e 's|@''HAVE_DECL_GETDOMAINNAME''@|$(HAVE_DECL_GETDOMAINNAME)|g' \ -e 's|@''HAVE_DECL_GETLOGIN_R''@|$(HAVE_DECL_GETLOGIN_R)|g' \ -e 's|@''HAVE_DECL_GETPAGESIZE''@|$(HAVE_DECL_GETPAGESIZE)|g' \ -e 's|@''HAVE_DECL_GETUSERSHELL''@|$(HAVE_DECL_GETUSERSHELL)|g' \ -e 's|@''HAVE_DECL_SETHOSTNAME''@|$(HAVE_DECL_SETHOSTNAME)|g' \ -e 's|@''HAVE_DECL_TTYNAME_R''@|$(HAVE_DECL_TTYNAME_R)|g' \ -e 's|@''HAVE_OS_H''@|$(HAVE_OS_H)|g' \ -e 's|@''HAVE_SYS_PARAM_H''@|$(HAVE_SYS_PARAM_H)|g' \ | \ sed -e 's|@''REPLACE_CHOWN''@|$(REPLACE_CHOWN)|g' \ -e 's|@''REPLACE_CLOSE''@|$(REPLACE_CLOSE)|g' \ -e 's|@''REPLACE_DUP''@|$(REPLACE_DUP)|g' \ -e 's|@''REPLACE_DUP2''@|$(REPLACE_DUP2)|g' \ -e 's|@''REPLACE_FCHOWNAT''@|$(REPLACE_FCHOWNAT)|g' \ -e 's|@''REPLACE_FTRUNCATE''@|$(REPLACE_FTRUNCATE)|g' \ -e 's|@''REPLACE_GETCWD''@|$(REPLACE_GETCWD)|g' \ -e 's|@''REPLACE_GETDOMAINNAME''@|$(REPLACE_GETDOMAINNAME)|g' \ -e 's|@''REPLACE_GETDTABLESIZE''@|$(REPLACE_GETDTABLESIZE)|g' \ -e 's|@''REPLACE_GETLOGIN_R''@|$(REPLACE_GETLOGIN_R)|g' \ -e 's|@''REPLACE_GETGROUPS''@|$(REPLACE_GETGROUPS)|g' \ -e 's|@''REPLACE_GETPAGESIZE''@|$(REPLACE_GETPAGESIZE)|g' \ -e 's|@''REPLACE_ISATTY''@|$(REPLACE_ISATTY)|g' \ -e 's|@''REPLACE_LCHOWN''@|$(REPLACE_LCHOWN)|g' \ -e 's|@''REPLACE_LINK''@|$(REPLACE_LINK)|g' \ -e 's|@''REPLACE_LINKAT''@|$(REPLACE_LINKAT)|g' \ -e 's|@''REPLACE_LSEEK''@|$(REPLACE_LSEEK)|g' \ -e 's|@''REPLACE_PREAD''@|$(REPLACE_PREAD)|g' \ -e 's|@''REPLACE_PWRITE''@|$(REPLACE_PWRITE)|g' \ -e 's|@''REPLACE_READ''@|$(REPLACE_READ)|g' \ -e 's|@''REPLACE_READLINK''@|$(REPLACE_READLINK)|g' \ -e 's|@''REPLACE_READLINKAT''@|$(REPLACE_READLINKAT)|g' \ -e 's|@''REPLACE_RMDIR''@|$(REPLACE_RMDIR)|g' \ -e 's|@''REPLACE_SLEEP''@|$(REPLACE_SLEEP)|g' \ -e 's|@''REPLACE_SYMLINK''@|$(REPLACE_SYMLINK)|g' \ -e 's|@''REPLACE_SYMLINKAT''@|$(REPLACE_SYMLINKAT)|g' \ -e 's|@''REPLACE_TTYNAME_R''@|$(REPLACE_TTYNAME_R)|g' \ -e 's|@''REPLACE_UNLINK''@|$(REPLACE_UNLINK)|g' \ -e 's|@''REPLACE_UNLINKAT''@|$(REPLACE_UNLINKAT)|g' \ -e 's|@''REPLACE_USLEEP''@|$(REPLACE_USLEEP)|g' \ -e 's|@''REPLACE_WRITE''@|$(REPLACE_WRITE)|g' \ -e 's|@''UNISTD_H_HAVE_WINSOCK2_H''@|$(UNISTD_H_HAVE_WINSOCK2_H)|g' \ -e 's|@''UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS''@|$(UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += unistd.h unistd.h-t EXTRA_DIST += unistd.in.h ## end gnulib module unistd ## begin gnulib module vasnprintf EXTRA_DIST += asnprintf.c float+.h printf-args.c printf-args.h printf-parse.c printf-parse.h vasnprintf.c vasnprintf.h EXTRA_libgnu_la_SOURCES += asnprintf.c printf-args.c printf-parse.c vasnprintf.c ## end gnulib module vasnprintf ## begin gnulib module verify EXTRA_DIST += verify.h ## end gnulib module verify ## begin gnulib module vsnprintf EXTRA_DIST += vsnprintf.c EXTRA_libgnu_la_SOURCES += vsnprintf.c ## end gnulib module vsnprintf ## begin gnulib module wchar BUILT_SOURCES += wchar.h # We need the following in order to create when the system # version does not work standalone. wchar.h: wchar.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''HAVE_FEATURES_H''@|$(HAVE_FEATURES_H)|g' \ -e 's|@''NEXT_WCHAR_H''@|$(NEXT_WCHAR_H)|g' \ -e 's|@''HAVE_WCHAR_H''@|$(HAVE_WCHAR_H)|g' \ -e 's/@''GNULIB_BTOWC''@/$(GNULIB_BTOWC)/g' \ -e 's/@''GNULIB_WCTOB''@/$(GNULIB_WCTOB)/g' \ -e 's/@''GNULIB_MBSINIT''@/$(GNULIB_MBSINIT)/g' \ -e 's/@''GNULIB_MBRTOWC''@/$(GNULIB_MBRTOWC)/g' \ -e 's/@''GNULIB_MBRLEN''@/$(GNULIB_MBRLEN)/g' \ -e 's/@''GNULIB_MBSRTOWCS''@/$(GNULIB_MBSRTOWCS)/g' \ -e 's/@''GNULIB_MBSNRTOWCS''@/$(GNULIB_MBSNRTOWCS)/g' \ -e 's/@''GNULIB_WCRTOMB''@/$(GNULIB_WCRTOMB)/g' \ -e 's/@''GNULIB_WCSRTOMBS''@/$(GNULIB_WCSRTOMBS)/g' \ -e 's/@''GNULIB_WCSNRTOMBS''@/$(GNULIB_WCSNRTOMBS)/g' \ -e 's/@''GNULIB_WCWIDTH''@/$(GNULIB_WCWIDTH)/g' \ -e 's/@''GNULIB_WMEMCHR''@/$(GNULIB_WMEMCHR)/g' \ -e 's/@''GNULIB_WMEMCMP''@/$(GNULIB_WMEMCMP)/g' \ -e 's/@''GNULIB_WMEMCPY''@/$(GNULIB_WMEMCPY)/g' \ -e 's/@''GNULIB_WMEMMOVE''@/$(GNULIB_WMEMMOVE)/g' \ -e 's/@''GNULIB_WMEMSET''@/$(GNULIB_WMEMSET)/g' \ -e 's/@''GNULIB_WCSLEN''@/$(GNULIB_WCSLEN)/g' \ -e 's/@''GNULIB_WCSNLEN''@/$(GNULIB_WCSNLEN)/g' \ -e 's/@''GNULIB_WCSCPY''@/$(GNULIB_WCSCPY)/g' \ -e 's/@''GNULIB_WCPCPY''@/$(GNULIB_WCPCPY)/g' \ -e 's/@''GNULIB_WCSNCPY''@/$(GNULIB_WCSNCPY)/g' \ -e 's/@''GNULIB_WCPNCPY''@/$(GNULIB_WCPNCPY)/g' \ -e 's/@''GNULIB_WCSCAT''@/$(GNULIB_WCSCAT)/g' \ -e 's/@''GNULIB_WCSNCAT''@/$(GNULIB_WCSNCAT)/g' \ -e 's/@''GNULIB_WCSCMP''@/$(GNULIB_WCSCMP)/g' \ -e 's/@''GNULIB_WCSNCMP''@/$(GNULIB_WCSNCMP)/g' \ -e 's/@''GNULIB_WCSCASECMP''@/$(GNULIB_WCSCASECMP)/g' \ -e 's/@''GNULIB_WCSNCASECMP''@/$(GNULIB_WCSNCASECMP)/g' \ -e 's/@''GNULIB_WCSCOLL''@/$(GNULIB_WCSCOLL)/g' \ -e 's/@''GNULIB_WCSXFRM''@/$(GNULIB_WCSXFRM)/g' \ -e 's/@''GNULIB_WCSDUP''@/$(GNULIB_WCSDUP)/g' \ -e 's/@''GNULIB_WCSCHR''@/$(GNULIB_WCSCHR)/g' \ -e 's/@''GNULIB_WCSRCHR''@/$(GNULIB_WCSRCHR)/g' \ -e 's/@''GNULIB_WCSCSPN''@/$(GNULIB_WCSCSPN)/g' \ -e 's/@''GNULIB_WCSSPN''@/$(GNULIB_WCSSPN)/g' \ -e 's/@''GNULIB_WCSPBRK''@/$(GNULIB_WCSPBRK)/g' \ -e 's/@''GNULIB_WCSSTR''@/$(GNULIB_WCSSTR)/g' \ -e 's/@''GNULIB_WCSTOK''@/$(GNULIB_WCSTOK)/g' \ -e 's/@''GNULIB_WCSWIDTH''@/$(GNULIB_WCSWIDTH)/g' \ < $(srcdir)/wchar.in.h | \ sed -e 's|@''HAVE_WINT_T''@|$(HAVE_WINT_T)|g' \ -e 's|@''HAVE_BTOWC''@|$(HAVE_BTOWC)|g' \ -e 's|@''HAVE_MBSINIT''@|$(HAVE_MBSINIT)|g' \ -e 's|@''HAVE_MBRTOWC''@|$(HAVE_MBRTOWC)|g' \ -e 's|@''HAVE_MBRLEN''@|$(HAVE_MBRLEN)|g' \ -e 's|@''HAVE_MBSRTOWCS''@|$(HAVE_MBSRTOWCS)|g' \ -e 's|@''HAVE_MBSNRTOWCS''@|$(HAVE_MBSNRTOWCS)|g' \ -e 's|@''HAVE_WCRTOMB''@|$(HAVE_WCRTOMB)|g' \ -e 's|@''HAVE_WCSRTOMBS''@|$(HAVE_WCSRTOMBS)|g' \ -e 's|@''HAVE_WCSNRTOMBS''@|$(HAVE_WCSNRTOMBS)|g' \ -e 's|@''HAVE_WMEMCHR''@|$(HAVE_WMEMCHR)|g' \ -e 's|@''HAVE_WMEMCMP''@|$(HAVE_WMEMCMP)|g' \ -e 's|@''HAVE_WMEMCPY''@|$(HAVE_WMEMCPY)|g' \ -e 's|@''HAVE_WMEMMOVE''@|$(HAVE_WMEMMOVE)|g' \ -e 's|@''HAVE_WMEMSET''@|$(HAVE_WMEMSET)|g' \ -e 's|@''HAVE_WCSLEN''@|$(HAVE_WCSLEN)|g' \ -e 's|@''HAVE_WCSNLEN''@|$(HAVE_WCSNLEN)|g' \ -e 's|@''HAVE_WCSCPY''@|$(HAVE_WCSCPY)|g' \ -e 's|@''HAVE_WCPCPY''@|$(HAVE_WCPCPY)|g' \ -e 's|@''HAVE_WCSNCPY''@|$(HAVE_WCSNCPY)|g' \ -e 's|@''HAVE_WCPNCPY''@|$(HAVE_WCPNCPY)|g' \ -e 's|@''HAVE_WCSCAT''@|$(HAVE_WCSCAT)|g' \ -e 's|@''HAVE_WCSNCAT''@|$(HAVE_WCSNCAT)|g' \ -e 's|@''HAVE_WCSCMP''@|$(HAVE_WCSCMP)|g' \ -e 's|@''HAVE_WCSNCMP''@|$(HAVE_WCSNCMP)|g' \ -e 's|@''HAVE_WCSCASECMP''@|$(HAVE_WCSCASECMP)|g' \ -e 's|@''HAVE_WCSNCASECMP''@|$(HAVE_WCSNCASECMP)|g' \ -e 's|@''HAVE_WCSCOLL''@|$(HAVE_WCSCOLL)|g' \ -e 's|@''HAVE_WCSXFRM''@|$(HAVE_WCSXFRM)|g' \ -e 's|@''HAVE_WCSDUP''@|$(HAVE_WCSDUP)|g' \ -e 's|@''HAVE_WCSCHR''@|$(HAVE_WCSCHR)|g' \ -e 's|@''HAVE_WCSRCHR''@|$(HAVE_WCSRCHR)|g' \ -e 's|@''HAVE_WCSCSPN''@|$(HAVE_WCSCSPN)|g' \ -e 's|@''HAVE_WCSSPN''@|$(HAVE_WCSSPN)|g' \ -e 's|@''HAVE_WCSPBRK''@|$(HAVE_WCSPBRK)|g' \ -e 's|@''HAVE_WCSSTR''@|$(HAVE_WCSSTR)|g' \ -e 's|@''HAVE_WCSTOK''@|$(HAVE_WCSTOK)|g' \ -e 's|@''HAVE_WCSWIDTH''@|$(HAVE_WCSWIDTH)|g' \ -e 's|@''HAVE_DECL_WCTOB''@|$(HAVE_DECL_WCTOB)|g' \ -e 's|@''HAVE_DECL_WCWIDTH''@|$(HAVE_DECL_WCWIDTH)|g' \ | \ sed -e 's|@''REPLACE_MBSTATE_T''@|$(REPLACE_MBSTATE_T)|g' \ -e 's|@''REPLACE_BTOWC''@|$(REPLACE_BTOWC)|g' \ -e 's|@''REPLACE_WCTOB''@|$(REPLACE_WCTOB)|g' \ -e 's|@''REPLACE_MBSINIT''@|$(REPLACE_MBSINIT)|g' \ -e 's|@''REPLACE_MBRTOWC''@|$(REPLACE_MBRTOWC)|g' \ -e 's|@''REPLACE_MBRLEN''@|$(REPLACE_MBRLEN)|g' \ -e 's|@''REPLACE_MBSRTOWCS''@|$(REPLACE_MBSRTOWCS)|g' \ -e 's|@''REPLACE_MBSNRTOWCS''@|$(REPLACE_MBSNRTOWCS)|g' \ -e 's|@''REPLACE_WCRTOMB''@|$(REPLACE_WCRTOMB)|g' \ -e 's|@''REPLACE_WCSRTOMBS''@|$(REPLACE_WCSRTOMBS)|g' \ -e 's|@''REPLACE_WCSNRTOMBS''@|$(REPLACE_WCSNRTOMBS)|g' \ -e 's|@''REPLACE_WCWIDTH''@|$(REPLACE_WCWIDTH)|g' \ -e 's|@''REPLACE_WCSWIDTH''@|$(REPLACE_WCSWIDTH)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += wchar.h wchar.h-t EXTRA_DIST += wchar.in.h ## end gnulib module wchar ## begin gnulib module wcrtomb EXTRA_DIST += wcrtomb.c EXTRA_libgnu_la_SOURCES += wcrtomb.c ## end gnulib module wcrtomb ## begin gnulib module wctype-h BUILT_SOURCES += wctype.h libgnu_la_SOURCES += wctype-h.c # We need the following in order to create when the system # doesn't have one that works with the given compiler. wctype.h: wctype.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's/@''HAVE_WCTYPE_H''@/$(HAVE_WCTYPE_H)/g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_WCTYPE_H''@|$(NEXT_WCTYPE_H)|g' \ -e 's/@''GNULIB_ISWBLANK''@/$(GNULIB_ISWBLANK)/g' \ -e 's/@''GNULIB_WCTYPE''@/$(GNULIB_WCTYPE)/g' \ -e 's/@''GNULIB_ISWCTYPE''@/$(GNULIB_ISWCTYPE)/g' \ -e 's/@''GNULIB_WCTRANS''@/$(GNULIB_WCTRANS)/g' \ -e 's/@''GNULIB_TOWCTRANS''@/$(GNULIB_TOWCTRANS)/g' \ -e 's/@''HAVE_ISWBLANK''@/$(HAVE_ISWBLANK)/g' \ -e 's/@''HAVE_ISWCNTRL''@/$(HAVE_ISWCNTRL)/g' \ -e 's/@''HAVE_WCTYPE_T''@/$(HAVE_WCTYPE_T)/g' \ -e 's/@''HAVE_WCTRANS_T''@/$(HAVE_WCTRANS_T)/g' \ -e 's/@''HAVE_WINT_T''@/$(HAVE_WINT_T)/g' \ -e 's/@''REPLACE_ISWBLANK''@/$(REPLACE_ISWBLANK)/g' \ -e 's/@''REPLACE_ISWCNTRL''@/$(REPLACE_ISWCNTRL)/g' \ -e 's/@''REPLACE_TOWLOWER''@/$(REPLACE_TOWLOWER)/g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/wctype.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += wctype.h wctype.h-t EXTRA_DIST += wctype.in.h ## end gnulib module wctype-h ## begin gnulib module xsize libgnu_la_SOURCES += xsize.h xsize.c ## end gnulib module xsize mostlyclean-local: mostlyclean-generic @for dir in '' $(MOSTLYCLEANDIRS); do \ if test -n "$$dir" && test -d $$dir; then \ echo "rmdir $$dir"; rmdir $$dir; \ fi; \ done; \ : gnuastro-0.2.33-8a3b/bootstrapped/lib/glthread/0000755000175000017500000000000013004464723016246 500000000000000gnuastro-0.2.33-8a3b/bootstrapped/lib/glthread/threadlib.c0000644000175000017500000000353613004436754020302 00000000000000/* Multithreading primitives. Copyright (C) 2005-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible , 2005. */ #include /* ========================================================================= */ #if USE_POSIX_THREADS /* Use the POSIX threads library. */ # include # include # if PTHREAD_IN_USE_DETECTION_HARD /* The function to be executed by a dummy thread. */ static void * dummy_thread_func (void *arg) { return arg; } int glthread_in_use (void) { static int tested; static int result; /* 1: linked with -lpthread, 0: only with libc */ if (!tested) { pthread_t thread; if (pthread_create (&thread, NULL, dummy_thread_func, NULL) != 0) /* Thread creation failed. */ result = 0; else { /* Thread creation works. */ void *retval; if (pthread_join (thread, &retval) != 0) abort (); result = 1; } tested = 1; } return result; } # endif #endif /* ========================================================================= */ /* This declaration is solely to ensure that after preprocessing this file is never empty. */ typedef int dummy; gnuastro-0.2.33-8a3b/bootstrapped/lib/glthread/lock.c0000644000175000017500000006417013004436754017275 00000000000000/* Locking in multithreaded situations. Copyright (C) 2005-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible , 2005. Based on GCC's gthr-posix.h, gthr-posix95.h, gthr-solaris.h, gthr-win32.h. */ #include #include "glthread/lock.h" /* ========================================================================= */ #if USE_POSIX_THREADS /* -------------------------- gl_lock_t datatype -------------------------- */ /* ------------------------- gl_rwlock_t datatype ------------------------- */ # if HAVE_PTHREAD_RWLOCK # if !defined PTHREAD_RWLOCK_INITIALIZER int glthread_rwlock_init_multithreaded (gl_rwlock_t *lock) { int err; err = pthread_rwlock_init (&lock->rwlock, NULL); if (err != 0) return err; lock->initialized = 1; return 0; } int glthread_rwlock_rdlock_multithreaded (gl_rwlock_t *lock) { if (!lock->initialized) { int err; err = pthread_mutex_lock (&lock->guard); if (err != 0) return err; if (!lock->initialized) { err = glthread_rwlock_init_multithreaded (lock); if (err != 0) { pthread_mutex_unlock (&lock->guard); return err; } } err = pthread_mutex_unlock (&lock->guard); if (err != 0) return err; } return pthread_rwlock_rdlock (&lock->rwlock); } int glthread_rwlock_wrlock_multithreaded (gl_rwlock_t *lock) { if (!lock->initialized) { int err; err = pthread_mutex_lock (&lock->guard); if (err != 0) return err; if (!lock->initialized) { err = glthread_rwlock_init_multithreaded (lock); if (err != 0) { pthread_mutex_unlock (&lock->guard); return err; } } err = pthread_mutex_unlock (&lock->guard); if (err != 0) return err; } return pthread_rwlock_wrlock (&lock->rwlock); } int glthread_rwlock_unlock_multithreaded (gl_rwlock_t *lock) { if (!lock->initialized) return EINVAL; return pthread_rwlock_unlock (&lock->rwlock); } int glthread_rwlock_destroy_multithreaded (gl_rwlock_t *lock) { int err; if (!lock->initialized) return EINVAL; err = pthread_rwlock_destroy (&lock->rwlock); if (err != 0) return err; lock->initialized = 0; return 0; } # endif # else int glthread_rwlock_init_multithreaded (gl_rwlock_t *lock) { int err; err = pthread_mutex_init (&lock->lock, NULL); if (err != 0) return err; err = pthread_cond_init (&lock->waiting_readers, NULL); if (err != 0) return err; err = pthread_cond_init (&lock->waiting_writers, NULL); if (err != 0) return err; lock->waiting_writers_count = 0; lock->runcount = 0; return 0; } int glthread_rwlock_rdlock_multithreaded (gl_rwlock_t *lock) { int err; err = pthread_mutex_lock (&lock->lock); if (err != 0) return err; /* Test whether only readers are currently running, and whether the runcount field will not overflow. */ /* POSIX says: "It is implementation-defined whether the calling thread acquires the lock when a writer does not hold the lock and there are writers blocked on the lock." Let's say, no: give the writers a higher priority. */ while (!(lock->runcount + 1 > 0 && lock->waiting_writers_count == 0)) { /* This thread has to wait for a while. Enqueue it among the waiting_readers. */ err = pthread_cond_wait (&lock->waiting_readers, &lock->lock); if (err != 0) { pthread_mutex_unlock (&lock->lock); return err; } } lock->runcount++; return pthread_mutex_unlock (&lock->lock); } int glthread_rwlock_wrlock_multithreaded (gl_rwlock_t *lock) { int err; err = pthread_mutex_lock (&lock->lock); if (err != 0) return err; /* Test whether no readers or writers are currently running. */ while (!(lock->runcount == 0)) { /* This thread has to wait for a while. Enqueue it among the waiting_writers. */ lock->waiting_writers_count++; err = pthread_cond_wait (&lock->waiting_writers, &lock->lock); if (err != 0) { lock->waiting_writers_count--; pthread_mutex_unlock (&lock->lock); return err; } lock->waiting_writers_count--; } lock->runcount--; /* runcount becomes -1 */ return pthread_mutex_unlock (&lock->lock); } int glthread_rwlock_unlock_multithreaded (gl_rwlock_t *lock) { int err; err = pthread_mutex_lock (&lock->lock); if (err != 0) return err; if (lock->runcount < 0) { /* Drop a writer lock. */ if (!(lock->runcount == -1)) { pthread_mutex_unlock (&lock->lock); return EINVAL; } lock->runcount = 0; } else { /* Drop a reader lock. */ if (!(lock->runcount > 0)) { pthread_mutex_unlock (&lock->lock); return EINVAL; } lock->runcount--; } if (lock->runcount == 0) { /* POSIX recommends that "write locks shall take precedence over read locks", to avoid "writer starvation". */ if (lock->waiting_writers_count > 0) { /* Wake up one of the waiting writers. */ err = pthread_cond_signal (&lock->waiting_writers); if (err != 0) { pthread_mutex_unlock (&lock->lock); return err; } } else { /* Wake up all waiting readers. */ err = pthread_cond_broadcast (&lock->waiting_readers); if (err != 0) { pthread_mutex_unlock (&lock->lock); return err; } } } return pthread_mutex_unlock (&lock->lock); } int glthread_rwlock_destroy_multithreaded (gl_rwlock_t *lock) { int err; err = pthread_mutex_destroy (&lock->lock); if (err != 0) return err; err = pthread_cond_destroy (&lock->waiting_readers); if (err != 0) return err; err = pthread_cond_destroy (&lock->waiting_writers); if (err != 0) return err; return 0; } # endif /* --------------------- gl_recursive_lock_t datatype --------------------- */ # if HAVE_PTHREAD_MUTEX_RECURSIVE # if defined PTHREAD_RECURSIVE_MUTEX_INITIALIZER || defined PTHREAD_RECURSIVE_MUTEX_INITIALIZER_NP int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock) { pthread_mutexattr_t attributes; int err; err = pthread_mutexattr_init (&attributes); if (err != 0) return err; err = pthread_mutexattr_settype (&attributes, PTHREAD_MUTEX_RECURSIVE); if (err != 0) { pthread_mutexattr_destroy (&attributes); return err; } err = pthread_mutex_init (lock, &attributes); if (err != 0) { pthread_mutexattr_destroy (&attributes); return err; } err = pthread_mutexattr_destroy (&attributes); if (err != 0) return err; return 0; } # else int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock) { pthread_mutexattr_t attributes; int err; err = pthread_mutexattr_init (&attributes); if (err != 0) return err; err = pthread_mutexattr_settype (&attributes, PTHREAD_MUTEX_RECURSIVE); if (err != 0) { pthread_mutexattr_destroy (&attributes); return err; } err = pthread_mutex_init (&lock->recmutex, &attributes); if (err != 0) { pthread_mutexattr_destroy (&attributes); return err; } err = pthread_mutexattr_destroy (&attributes); if (err != 0) return err; lock->initialized = 1; return 0; } int glthread_recursive_lock_lock_multithreaded (gl_recursive_lock_t *lock) { if (!lock->initialized) { int err; err = pthread_mutex_lock (&lock->guard); if (err != 0) return err; if (!lock->initialized) { err = glthread_recursive_lock_init_multithreaded (lock); if (err != 0) { pthread_mutex_unlock (&lock->guard); return err; } } err = pthread_mutex_unlock (&lock->guard); if (err != 0) return err; } return pthread_mutex_lock (&lock->recmutex); } int glthread_recursive_lock_unlock_multithreaded (gl_recursive_lock_t *lock) { if (!lock->initialized) return EINVAL; return pthread_mutex_unlock (&lock->recmutex); } int glthread_recursive_lock_destroy_multithreaded (gl_recursive_lock_t *lock) { int err; if (!lock->initialized) return EINVAL; err = pthread_mutex_destroy (&lock->recmutex); if (err != 0) return err; lock->initialized = 0; return 0; } # endif # else int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock) { int err; err = pthread_mutex_init (&lock->mutex, NULL); if (err != 0) return err; lock->owner = (pthread_t) 0; lock->depth = 0; return 0; } int glthread_recursive_lock_lock_multithreaded (gl_recursive_lock_t *lock) { pthread_t self = pthread_self (); if (lock->owner != self) { int err; err = pthread_mutex_lock (&lock->mutex); if (err != 0) return err; lock->owner = self; } if (++(lock->depth) == 0) /* wraparound? */ { lock->depth--; return EAGAIN; } return 0; } int glthread_recursive_lock_unlock_multithreaded (gl_recursive_lock_t *lock) { if (lock->owner != pthread_self ()) return EPERM; if (lock->depth == 0) return EINVAL; if (--(lock->depth) == 0) { lock->owner = (pthread_t) 0; return pthread_mutex_unlock (&lock->mutex); } else return 0; } int glthread_recursive_lock_destroy_multithreaded (gl_recursive_lock_t *lock) { if (lock->owner != (pthread_t) 0) return EBUSY; return pthread_mutex_destroy (&lock->mutex); } # endif /* -------------------------- gl_once_t datatype -------------------------- */ static const pthread_once_t fresh_once = PTHREAD_ONCE_INIT; int glthread_once_singlethreaded (pthread_once_t *once_control) { /* We don't know whether pthread_once_t is an integer type, a floating-point type, a pointer type, or a structure type. */ char *firstbyte = (char *)once_control; if (*firstbyte == *(const char *)&fresh_once) { /* First time use of once_control. Invert the first byte. */ *firstbyte = ~ *(const char *)&fresh_once; return 1; } else return 0; } #endif /* ========================================================================= */ #if USE_PTH_THREADS /* Use the GNU Pth threads library. */ /* -------------------------- gl_lock_t datatype -------------------------- */ /* ------------------------- gl_rwlock_t datatype ------------------------- */ /* --------------------- gl_recursive_lock_t datatype --------------------- */ /* -------------------------- gl_once_t datatype -------------------------- */ static void glthread_once_call (void *arg) { void (**gl_once_temp_addr) (void) = (void (**) (void)) arg; void (*initfunction) (void) = *gl_once_temp_addr; initfunction (); } int glthread_once_multithreaded (pth_once_t *once_control, void (*initfunction) (void)) { void (*temp) (void) = initfunction; return (!pth_once (once_control, glthread_once_call, &temp) ? errno : 0); } int glthread_once_singlethreaded (pth_once_t *once_control) { /* We know that pth_once_t is an integer type. */ if (*once_control == PTH_ONCE_INIT) { /* First time use of once_control. Invert the marker. */ *once_control = ~ PTH_ONCE_INIT; return 1; } else return 0; } #endif /* ========================================================================= */ #if USE_SOLARIS_THREADS /* Use the old Solaris threads library. */ /* -------------------------- gl_lock_t datatype -------------------------- */ /* ------------------------- gl_rwlock_t datatype ------------------------- */ /* --------------------- gl_recursive_lock_t datatype --------------------- */ int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock) { int err; err = mutex_init (&lock->mutex, USYNC_THREAD, NULL); if (err != 0) return err; lock->owner = (thread_t) 0; lock->depth = 0; return 0; } int glthread_recursive_lock_lock_multithreaded (gl_recursive_lock_t *lock) { thread_t self = thr_self (); if (lock->owner != self) { int err; err = mutex_lock (&lock->mutex); if (err != 0) return err; lock->owner = self; } if (++(lock->depth) == 0) /* wraparound? */ { lock->depth--; return EAGAIN; } return 0; } int glthread_recursive_lock_unlock_multithreaded (gl_recursive_lock_t *lock) { if (lock->owner != thr_self ()) return EPERM; if (lock->depth == 0) return EINVAL; if (--(lock->depth) == 0) { lock->owner = (thread_t) 0; return mutex_unlock (&lock->mutex); } else return 0; } int glthread_recursive_lock_destroy_multithreaded (gl_recursive_lock_t *lock) { if (lock->owner != (thread_t) 0) return EBUSY; return mutex_destroy (&lock->mutex); } /* -------------------------- gl_once_t datatype -------------------------- */ int glthread_once_multithreaded (gl_once_t *once_control, void (*initfunction) (void)) { if (!once_control->inited) { int err; /* Use the mutex to guarantee that if another thread is already calling the initfunction, this thread waits until it's finished. */ err = mutex_lock (&once_control->mutex); if (err != 0) return err; if (!once_control->inited) { once_control->inited = 1; initfunction (); } return mutex_unlock (&once_control->mutex); } else return 0; } int glthread_once_singlethreaded (gl_once_t *once_control) { /* We know that gl_once_t contains an integer type. */ if (!once_control->inited) { /* First time use of once_control. Invert the marker. */ once_control->inited = ~ 0; return 1; } else return 0; } #endif /* ========================================================================= */ #if USE_WINDOWS_THREADS /* -------------------------- gl_lock_t datatype -------------------------- */ void glthread_lock_init_func (gl_lock_t *lock) { InitializeCriticalSection (&lock->lock); lock->guard.done = 1; } int glthread_lock_lock_func (gl_lock_t *lock) { if (!lock->guard.done) { if (InterlockedIncrement (&lock->guard.started) == 0) /* This thread is the first one to need this lock. Initialize it. */ glthread_lock_init (lock); else /* Yield the CPU while waiting for another thread to finish initializing this lock. */ while (!lock->guard.done) Sleep (0); } EnterCriticalSection (&lock->lock); return 0; } int glthread_lock_unlock_func (gl_lock_t *lock) { if (!lock->guard.done) return EINVAL; LeaveCriticalSection (&lock->lock); return 0; } int glthread_lock_destroy_func (gl_lock_t *lock) { if (!lock->guard.done) return EINVAL; DeleteCriticalSection (&lock->lock); lock->guard.done = 0; return 0; } /* ------------------------- gl_rwlock_t datatype ------------------------- */ /* In this file, the waitqueues are implemented as circular arrays. */ #define gl_waitqueue_t gl_carray_waitqueue_t static void gl_waitqueue_init (gl_waitqueue_t *wq) { wq->array = NULL; wq->count = 0; wq->alloc = 0; wq->offset = 0; } /* Enqueues the current thread, represented by an event, in a wait queue. Returns INVALID_HANDLE_VALUE if an allocation failure occurs. */ static HANDLE gl_waitqueue_add (gl_waitqueue_t *wq) { HANDLE event; unsigned int index; if (wq->count == wq->alloc) { unsigned int new_alloc = 2 * wq->alloc + 1; HANDLE *new_array = (HANDLE *) realloc (wq->array, new_alloc * sizeof (HANDLE)); if (new_array == NULL) /* No more memory. */ return INVALID_HANDLE_VALUE; /* Now is a good opportunity to rotate the array so that its contents starts at offset 0. */ if (wq->offset > 0) { unsigned int old_count = wq->count; unsigned int old_alloc = wq->alloc; unsigned int old_offset = wq->offset; unsigned int i; if (old_offset + old_count > old_alloc) { unsigned int limit = old_offset + old_count - old_alloc; for (i = 0; i < limit; i++) new_array[old_alloc + i] = new_array[i]; } for (i = 0; i < old_count; i++) new_array[i] = new_array[old_offset + i]; wq->offset = 0; } wq->array = new_array; wq->alloc = new_alloc; } /* Whether the created event is a manual-reset one or an auto-reset one, does not matter, since we will wait on it only once. */ event = CreateEvent (NULL, TRUE, FALSE, NULL); if (event == INVALID_HANDLE_VALUE) /* No way to allocate an event. */ return INVALID_HANDLE_VALUE; index = wq->offset + wq->count; if (index >= wq->alloc) index -= wq->alloc; wq->array[index] = event; wq->count++; return event; } /* Notifies the first thread from a wait queue and dequeues it. */ static void gl_waitqueue_notify_first (gl_waitqueue_t *wq) { SetEvent (wq->array[wq->offset + 0]); wq->offset++; wq->count--; if (wq->count == 0 || wq->offset == wq->alloc) wq->offset = 0; } /* Notifies all threads from a wait queue and dequeues them all. */ static void gl_waitqueue_notify_all (gl_waitqueue_t *wq) { unsigned int i; for (i = 0; i < wq->count; i++) { unsigned int index = wq->offset + i; if (index >= wq->alloc) index -= wq->alloc; SetEvent (wq->array[index]); } wq->count = 0; wq->offset = 0; } void glthread_rwlock_init_func (gl_rwlock_t *lock) { InitializeCriticalSection (&lock->lock); gl_waitqueue_init (&lock->waiting_readers); gl_waitqueue_init (&lock->waiting_writers); lock->runcount = 0; lock->guard.done = 1; } int glthread_rwlock_rdlock_func (gl_rwlock_t *lock) { if (!lock->guard.done) { if (InterlockedIncrement (&lock->guard.started) == 0) /* This thread is the first one to need this lock. Initialize it. */ glthread_rwlock_init (lock); else /* Yield the CPU while waiting for another thread to finish initializing this lock. */ while (!lock->guard.done) Sleep (0); } EnterCriticalSection (&lock->lock); /* Test whether only readers are currently running, and whether the runcount field will not overflow. */ if (!(lock->runcount + 1 > 0)) { /* This thread has to wait for a while. Enqueue it among the waiting_readers. */ HANDLE event = gl_waitqueue_add (&lock->waiting_readers); if (event != INVALID_HANDLE_VALUE) { DWORD result; LeaveCriticalSection (&lock->lock); /* Wait until another thread signals this event. */ result = WaitForSingleObject (event, INFINITE); if (result == WAIT_FAILED || result == WAIT_TIMEOUT) abort (); CloseHandle (event); /* The thread which signalled the event already did the bookkeeping: removed us from the waiting_readers, incremented lock->runcount. */ if (!(lock->runcount > 0)) abort (); return 0; } else { /* Allocation failure. Weird. */ do { LeaveCriticalSection (&lock->lock); Sleep (1); EnterCriticalSection (&lock->lock); } while (!(lock->runcount + 1 > 0)); } } lock->runcount++; LeaveCriticalSection (&lock->lock); return 0; } int glthread_rwlock_wrlock_func (gl_rwlock_t *lock) { if (!lock->guard.done) { if (InterlockedIncrement (&lock->guard.started) == 0) /* This thread is the first one to need this lock. Initialize it. */ glthread_rwlock_init (lock); else /* Yield the CPU while waiting for another thread to finish initializing this lock. */ while (!lock->guard.done) Sleep (0); } EnterCriticalSection (&lock->lock); /* Test whether no readers or writers are currently running. */ if (!(lock->runcount == 0)) { /* This thread has to wait for a while. Enqueue it among the waiting_writers. */ HANDLE event = gl_waitqueue_add (&lock->waiting_writers); if (event != INVALID_HANDLE_VALUE) { DWORD result; LeaveCriticalSection (&lock->lock); /* Wait until another thread signals this event. */ result = WaitForSingleObject (event, INFINITE); if (result == WAIT_FAILED || result == WAIT_TIMEOUT) abort (); CloseHandle (event); /* The thread which signalled the event already did the bookkeeping: removed us from the waiting_writers, set lock->runcount = -1. */ if (!(lock->runcount == -1)) abort (); return 0; } else { /* Allocation failure. Weird. */ do { LeaveCriticalSection (&lock->lock); Sleep (1); EnterCriticalSection (&lock->lock); } while (!(lock->runcount == 0)); } } lock->runcount--; /* runcount becomes -1 */ LeaveCriticalSection (&lock->lock); return 0; } int glthread_rwlock_unlock_func (gl_rwlock_t *lock) { if (!lock->guard.done) return EINVAL; EnterCriticalSection (&lock->lock); if (lock->runcount < 0) { /* Drop a writer lock. */ if (!(lock->runcount == -1)) abort (); lock->runcount = 0; } else { /* Drop a reader lock. */ if (!(lock->runcount > 0)) { LeaveCriticalSection (&lock->lock); return EPERM; } lock->runcount--; } if (lock->runcount == 0) { /* POSIX recommends that "write locks shall take precedence over read locks", to avoid "writer starvation". */ if (lock->waiting_writers.count > 0) { /* Wake up one of the waiting writers. */ lock->runcount--; gl_waitqueue_notify_first (&lock->waiting_writers); } else { /* Wake up all waiting readers. */ lock->runcount += lock->waiting_readers.count; gl_waitqueue_notify_all (&lock->waiting_readers); } } LeaveCriticalSection (&lock->lock); return 0; } int glthread_rwlock_destroy_func (gl_rwlock_t *lock) { if (!lock->guard.done) return EINVAL; if (lock->runcount != 0) return EBUSY; DeleteCriticalSection (&lock->lock); if (lock->waiting_readers.array != NULL) free (lock->waiting_readers.array); if (lock->waiting_writers.array != NULL) free (lock->waiting_writers.array); lock->guard.done = 0; return 0; } /* --------------------- gl_recursive_lock_t datatype --------------------- */ void glthread_recursive_lock_init_func (gl_recursive_lock_t *lock) { lock->owner = 0; lock->depth = 0; InitializeCriticalSection (&lock->lock); lock->guard.done = 1; } int glthread_recursive_lock_lock_func (gl_recursive_lock_t *lock) { if (!lock->guard.done) { if (InterlockedIncrement (&lock->guard.started) == 0) /* This thread is the first one to need this lock. Initialize it. */ glthread_recursive_lock_init (lock); else /* Yield the CPU while waiting for another thread to finish initializing this lock. */ while (!lock->guard.done) Sleep (0); } { DWORD self = GetCurrentThreadId (); if (lock->owner != self) { EnterCriticalSection (&lock->lock); lock->owner = self; } if (++(lock->depth) == 0) /* wraparound? */ { lock->depth--; return EAGAIN; } } return 0; } int glthread_recursive_lock_unlock_func (gl_recursive_lock_t *lock) { if (lock->owner != GetCurrentThreadId ()) return EPERM; if (lock->depth == 0) return EINVAL; if (--(lock->depth) == 0) { lock->owner = 0; LeaveCriticalSection (&lock->lock); } return 0; } int glthread_recursive_lock_destroy_func (gl_recursive_lock_t *lock) { if (lock->owner != 0) return EBUSY; DeleteCriticalSection (&lock->lock); lock->guard.done = 0; return 0; } /* -------------------------- gl_once_t datatype -------------------------- */ void glthread_once_func (gl_once_t *once_control, void (*initfunction) (void)) { if (once_control->inited <= 0) { if (InterlockedIncrement (&once_control->started) == 0) { /* This thread is the first one to come to this once_control. */ InitializeCriticalSection (&once_control->lock); EnterCriticalSection (&once_control->lock); once_control->inited = 0; initfunction (); once_control->inited = 1; LeaveCriticalSection (&once_control->lock); } else { /* Undo last operation. */ InterlockedDecrement (&once_control->started); /* Some other thread has already started the initialization. Yield the CPU while waiting for the other thread to finish initializing and taking the lock. */ while (once_control->inited < 0) Sleep (0); if (once_control->inited <= 0) { /* Take the lock. This blocks until the other thread has finished calling the initfunction. */ EnterCriticalSection (&once_control->lock); LeaveCriticalSection (&once_control->lock); if (!(once_control->inited > 0)) abort (); } } } } #endif /* ========================================================================= */ gnuastro-0.2.33-8a3b/bootstrapped/lib/glthread/lock.h0000644000175000017500000010665213004436754017304 00000000000000/* Locking in multithreaded situations. Copyright (C) 2005-2016 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible , 2005. Based on GCC's gthr-posix.h, gthr-posix95.h, gthr-solaris.h, gthr-win32.h. */ /* This file contains locking primitives for use with a given thread library. It does not contain primitives for creating threads or for other synchronization primitives. Normal (non-recursive) locks: Type: gl_lock_t Declaration: gl_lock_define(extern, name) Initializer: gl_lock_define_initialized(, name) Initialization: gl_lock_init (name); Taking the lock: gl_lock_lock (name); Releasing the lock: gl_lock_unlock (name); De-initialization: gl_lock_destroy (name); Equivalent functions with control of error handling: Initialization: err = glthread_lock_init (&name); Taking the lock: err = glthread_lock_lock (&name); Releasing the lock: err = glthread_lock_unlock (&name); De-initialization: err = glthread_lock_destroy (&name); Read-Write (non-recursive) locks: Type: gl_rwlock_t Declaration: gl_rwlock_define(extern, name) Initializer: gl_rwlock_define_initialized(, name) Initialization: gl_rwlock_init (name); Taking the lock: gl_rwlock_rdlock (name); gl_rwlock_wrlock (name); Releasing the lock: gl_rwlock_unlock (name); De-initialization: gl_rwlock_destroy (name); Equivalent functions with control of error handling: Initialization: err = glthread_rwlock_init (&name); Taking the lock: err = glthread_rwlock_rdlock (&name); err = glthread_rwlock_wrlock (&name); Releasing the lock: err = glthread_rwlock_unlock (&name); De-initialization: err = glthread_rwlock_destroy (&name); Recursive locks: Type: gl_recursive_lock_t Declaration: gl_recursive_lock_define(extern, name) Initializer: gl_recursive_lock_define_initialized(, name) Initialization: gl_recursive_lock_init (name); Taking the lock: gl_recursive_lock_lock (name); Releasing the lock: gl_recursive_lock_unlock (name); De-initialization: gl_recursive_lock_destroy (name); Equivalent functions with control of error handling: Initialization: err = glthread_recursive_lock_init (&name); Taking the lock: err = glthread_recursive_lock_lock (&name); Releasing the lock: err = glthread_recursive_lock_unlock (&name); De-initialization: err = glthread_recursive_lock_destroy (&name); Once-only execution: Type: gl_once_t Initializer: gl_once_define(extern, name) Execution: gl_once (name, initfunction); Equivalent functions with control of error handling: Execution: err = glthread_once (&name, initfunction); */ #ifndef _LOCK_H #define _LOCK_H #include #include /* ========================================================================= */ #if USE_POSIX_THREADS /* Use the POSIX threads library. */ # include # ifdef __cplusplus extern "C" { # endif # if PTHREAD_IN_USE_DETECTION_HARD /* The pthread_in_use() detection needs to be done at runtime. */ # define pthread_in_use() \ glthread_in_use () extern int glthread_in_use (void); # endif # if USE_POSIX_THREADS_WEAK /* Use weak references to the POSIX threads library. */ /* Weak references avoid dragging in external libraries if the other parts of the program don't use them. Here we use them, because we don't want every program that uses libintl to depend on libpthread. This assumes that libpthread would not be loaded after libintl; i.e. if libintl is loaded first, by an executable that does not depend on libpthread, and then a module is dynamically loaded that depends on libpthread, libintl will not be multithread-safe. */ /* The way to test at runtime whether libpthread is present is to test whether a function pointer's value, such as &pthread_mutex_init, is non-NULL. However, some versions of GCC have a bug through which, in PIC mode, &foo != NULL always evaluates to true if there is a direct call to foo(...) in the same function. To avoid this, we test the address of a function in libpthread that we don't use. */ # pragma weak pthread_mutex_init # pragma weak pthread_mutex_lock # pragma weak pthread_mutex_unlock # pragma weak pthread_mutex_destroy # pragma weak pthread_rwlock_init # pragma weak pthread_rwlock_rdlock # pragma weak pthread_rwlock_wrlock # pragma weak pthread_rwlock_unlock # pragma weak pthread_rwlock_destroy # pragma weak pthread_once # pragma weak pthread_cond_init # pragma weak pthread_cond_wait # pragma weak pthread_cond_signal # pragma weak pthread_cond_broadcast # pragma weak pthread_cond_destroy # pragma weak pthread_mutexattr_init # pragma weak pthread_mutexattr_settype # pragma weak pthread_mutexattr_destroy # ifndef pthread_self # pragma weak pthread_self # endif # if !PTHREAD_IN_USE_DETECTION_HARD # pragma weak pthread_cancel # define pthread_in_use() (pthread_cancel != NULL) # endif # else # if !PTHREAD_IN_USE_DETECTION_HARD # define pthread_in_use() 1 # endif # endif /* -------------------------- gl_lock_t datatype -------------------------- */ typedef pthread_mutex_t gl_lock_t; # define gl_lock_define(STORAGECLASS, NAME) \ STORAGECLASS pthread_mutex_t NAME; # define gl_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS pthread_mutex_t NAME = gl_lock_initializer; # define gl_lock_initializer \ PTHREAD_MUTEX_INITIALIZER # define glthread_lock_init(LOCK) \ (pthread_in_use () ? pthread_mutex_init (LOCK, NULL) : 0) # define glthread_lock_lock(LOCK) \ (pthread_in_use () ? pthread_mutex_lock (LOCK) : 0) # define glthread_lock_unlock(LOCK) \ (pthread_in_use () ? pthread_mutex_unlock (LOCK) : 0) # define glthread_lock_destroy(LOCK) \ (pthread_in_use () ? pthread_mutex_destroy (LOCK) : 0) /* ------------------------- gl_rwlock_t datatype ------------------------- */ # if HAVE_PTHREAD_RWLOCK # ifdef PTHREAD_RWLOCK_INITIALIZER typedef pthread_rwlock_t gl_rwlock_t; # define gl_rwlock_define(STORAGECLASS, NAME) \ STORAGECLASS pthread_rwlock_t NAME; # define gl_rwlock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS pthread_rwlock_t NAME = gl_rwlock_initializer; # define gl_rwlock_initializer \ PTHREAD_RWLOCK_INITIALIZER # define glthread_rwlock_init(LOCK) \ (pthread_in_use () ? pthread_rwlock_init (LOCK, NULL) : 0) # define glthread_rwlock_rdlock(LOCK) \ (pthread_in_use () ? pthread_rwlock_rdlock (LOCK) : 0) # define glthread_rwlock_wrlock(LOCK) \ (pthread_in_use () ? pthread_rwlock_wrlock (LOCK) : 0) # define glthread_rwlock_unlock(LOCK) \ (pthread_in_use () ? pthread_rwlock_unlock (LOCK) : 0) # define glthread_rwlock_destroy(LOCK) \ (pthread_in_use () ? pthread_rwlock_destroy (LOCK) : 0) # else typedef struct { int initialized; pthread_mutex_t guard; /* protects the initialization */ pthread_rwlock_t rwlock; /* read-write lock */ } gl_rwlock_t; # define gl_rwlock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_rwlock_t NAME; # define gl_rwlock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_rwlock_t NAME = gl_rwlock_initializer; # define gl_rwlock_initializer \ { 0, PTHREAD_MUTEX_INITIALIZER } # define glthread_rwlock_init(LOCK) \ (pthread_in_use () ? glthread_rwlock_init_multithreaded (LOCK) : 0) # define glthread_rwlock_rdlock(LOCK) \ (pthread_in_use () ? glthread_rwlock_rdlock_multithreaded (LOCK) : 0) # define glthread_rwlock_wrlock(LOCK) \ (pthread_in_use () ? glthread_rwlock_wrlock_multithreaded (LOCK) : 0) # define glthread_rwlock_unlock(LOCK) \ (pthread_in_use () ? glthread_rwlock_unlock_multithreaded (LOCK) : 0) # define glthread_rwlock_destroy(LOCK) \ (pthread_in_use () ? glthread_rwlock_destroy_multithreaded (LOCK) : 0) extern int glthread_rwlock_init_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_rdlock_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_wrlock_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_unlock_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_destroy_multithreaded (gl_rwlock_t *lock); # endif # else typedef struct { pthread_mutex_t lock; /* protects the remaining fields */ pthread_cond_t waiting_readers; /* waiting readers */ pthread_cond_t waiting_writers; /* waiting writers */ unsigned int waiting_writers_count; /* number of waiting writers */ int runcount; /* number of readers running, or -1 when a writer runs */ } gl_rwlock_t; # define gl_rwlock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_rwlock_t NAME; # define gl_rwlock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_rwlock_t NAME = gl_rwlock_initializer; # define gl_rwlock_initializer \ { PTHREAD_MUTEX_INITIALIZER, PTHREAD_COND_INITIALIZER, PTHREAD_COND_INITIALIZER, 0, 0 } # define glthread_rwlock_init(LOCK) \ (pthread_in_use () ? glthread_rwlock_init_multithreaded (LOCK) : 0) # define glthread_rwlock_rdlock(LOCK) \ (pthread_in_use () ? glthread_rwlock_rdlock_multithreaded (LOCK) : 0) # define glthread_rwlock_wrlock(LOCK) \ (pthread_in_use () ? glthread_rwlock_wrlock_multithreaded (LOCK) : 0) # define glthread_rwlock_unlock(LOCK) \ (pthread_in_use () ? glthread_rwlock_unlock_multithreaded (LOCK) : 0) # define glthread_rwlock_destroy(LOCK) \ (pthread_in_use () ? glthread_rwlock_destroy_multithreaded (LOCK) : 0) extern int glthread_rwlock_init_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_rdlock_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_wrlock_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_unlock_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_destroy_multithreaded (gl_rwlock_t *lock); # endif /* --------------------- gl_recursive_lock_t datatype --------------------- */ # if HAVE_PTHREAD_MUTEX_RECURSIVE # if defined PTHREAD_RECURSIVE_MUTEX_INITIALIZER || defined PTHREAD_RECURSIVE_MUTEX_INITIALIZER_NP typedef pthread_mutex_t gl_recursive_lock_t; # define gl_recursive_lock_define(STORAGECLASS, NAME) \ STORAGECLASS pthread_mutex_t NAME; # define gl_recursive_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS pthread_mutex_t NAME = gl_recursive_lock_initializer; # ifdef PTHREAD_RECURSIVE_MUTEX_INITIALIZER # define gl_recursive_lock_initializer \ PTHREAD_RECURSIVE_MUTEX_INITIALIZER # else # define gl_recursive_lock_initializer \ PTHREAD_RECURSIVE_MUTEX_INITIALIZER_NP # endif # define glthread_recursive_lock_init(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_init_multithreaded (LOCK) : 0) # define glthread_recursive_lock_lock(LOCK) \ (pthread_in_use () ? pthread_mutex_lock (LOCK) : 0) # define glthread_recursive_lock_unlock(LOCK) \ (pthread_in_use () ? pthread_mutex_unlock (LOCK) : 0) # define glthread_recursive_lock_destroy(LOCK) \ (pthread_in_use () ? pthread_mutex_destroy (LOCK) : 0) extern int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock); # else typedef struct { pthread_mutex_t recmutex; /* recursive mutex */ pthread_mutex_t guard; /* protects the initialization */ int initialized; } gl_recursive_lock_t; # define gl_recursive_lock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME; # define gl_recursive_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME = gl_recursive_lock_initializer; # define gl_recursive_lock_initializer \ { PTHREAD_MUTEX_INITIALIZER, PTHREAD_MUTEX_INITIALIZER, 0 } # define glthread_recursive_lock_init(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_init_multithreaded (LOCK) : 0) # define glthread_recursive_lock_lock(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_lock_multithreaded (LOCK) : 0) # define glthread_recursive_lock_unlock(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_unlock_multithreaded (LOCK) : 0) # define glthread_recursive_lock_destroy(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_destroy_multithreaded (LOCK) : 0) extern int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_lock_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_unlock_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_destroy_multithreaded (gl_recursive_lock_t *lock); # endif # else /* Old versions of POSIX threads on Solaris did not have recursive locks. We have to implement them ourselves. */ typedef struct { pthread_mutex_t mutex; pthread_t owner; unsigned long depth; } gl_recursive_lock_t; # define gl_recursive_lock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME; # define gl_recursive_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME = gl_recursive_lock_initializer; # define gl_recursive_lock_initializer \ { PTHREAD_MUTEX_INITIALIZER, (pthread_t) 0, 0 } # define glthread_recursive_lock_init(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_init_multithreaded (LOCK) : 0) # define glthread_recursive_lock_lock(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_lock_multithreaded (LOCK) : 0) # define glthread_recursive_lock_unlock(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_unlock_multithreaded (LOCK) : 0) # define glthread_recursive_lock_destroy(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_destroy_multithreaded (LOCK) : 0) extern int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_lock_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_unlock_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_destroy_multithreaded (gl_recursive_lock_t *lock); # endif /* -------------------------- gl_once_t datatype -------------------------- */ typedef pthread_once_t gl_once_t; # define gl_once_define(STORAGECLASS, NAME) \ STORAGECLASS pthread_once_t NAME = PTHREAD_ONCE_INIT; # define glthread_once(ONCE_CONTROL, INITFUNCTION) \ (pthread_in_use () \ ? pthread_once (ONCE_CONTROL, INITFUNCTION) \ : (glthread_once_singlethreaded (ONCE_CONTROL) ? (INITFUNCTION (), 0) : 0)) extern int glthread_once_singlethreaded (pthread_once_t *once_control); # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_PTH_THREADS /* Use the GNU Pth threads library. */ # include # ifdef __cplusplus extern "C" { # endif # if USE_PTH_THREADS_WEAK /* Use weak references to the GNU Pth threads library. */ # pragma weak pth_mutex_init # pragma weak pth_mutex_acquire # pragma weak pth_mutex_release # pragma weak pth_rwlock_init # pragma weak pth_rwlock_acquire # pragma weak pth_rwlock_release # pragma weak pth_once # pragma weak pth_cancel # define pth_in_use() (pth_cancel != NULL) # else # define pth_in_use() 1 # endif /* -------------------------- gl_lock_t datatype -------------------------- */ typedef pth_mutex_t gl_lock_t; # define gl_lock_define(STORAGECLASS, NAME) \ STORAGECLASS pth_mutex_t NAME; # define gl_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS pth_mutex_t NAME = gl_lock_initializer; # define gl_lock_initializer \ PTH_MUTEX_INIT # define glthread_lock_init(LOCK) \ (pth_in_use () && !pth_mutex_init (LOCK) ? errno : 0) # define glthread_lock_lock(LOCK) \ (pth_in_use () && !pth_mutex_acquire (LOCK, 0, NULL) ? errno : 0) # define glthread_lock_unlock(LOCK) \ (pth_in_use () && !pth_mutex_release (LOCK) ? errno : 0) # define glthread_lock_destroy(LOCK) \ ((void)(LOCK), 0) /* ------------------------- gl_rwlock_t datatype ------------------------- */ typedef pth_rwlock_t gl_rwlock_t; # define gl_rwlock_define(STORAGECLASS, NAME) \ STORAGECLASS pth_rwlock_t NAME; # define gl_rwlock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS pth_rwlock_t NAME = gl_rwlock_initializer; # define gl_rwlock_initializer \ PTH_RWLOCK_INIT # define glthread_rwlock_init(LOCK) \ (pth_in_use () && !pth_rwlock_init (LOCK) ? errno : 0) # define glthread_rwlock_rdlock(LOCK) \ (pth_in_use () && !pth_rwlock_acquire (LOCK, PTH_RWLOCK_RD, 0, NULL) ? errno : 0) # define glthread_rwlock_wrlock(LOCK) \ (pth_in_use () && !pth_rwlock_acquire (LOCK, PTH_RWLOCK_RW, 0, NULL) ? errno : 0) # define glthread_rwlock_unlock(LOCK) \ (pth_in_use () && !pth_rwlock_release (LOCK) ? errno : 0) # define glthread_rwlock_destroy(LOCK) \ ((void)(LOCK), 0) /* --------------------- gl_recursive_lock_t datatype --------------------- */ /* In Pth, mutexes are recursive by default. */ typedef pth_mutex_t gl_recursive_lock_t; # define gl_recursive_lock_define(STORAGECLASS, NAME) \ STORAGECLASS pth_mutex_t NAME; # define gl_recursive_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS pth_mutex_t NAME = gl_recursive_lock_initializer; # define gl_recursive_lock_initializer \ PTH_MUTEX_INIT # define glthread_recursive_lock_init(LOCK) \ (pth_in_use () && !pth_mutex_init (LOCK) ? errno : 0) # define glthread_recursive_lock_lock(LOCK) \ (pth_in_use () && !pth_mutex_acquire (LOCK, 0, NULL) ? errno : 0) # define glthread_recursive_lock_unlock(LOCK) \ (pth_in_use () && !pth_mutex_release (LOCK) ? errno : 0) # define glthread_recursive_lock_destroy(LOCK) \ ((void)(LOCK), 0) /* -------------------------- gl_once_t datatype -------------------------- */ typedef pth_once_t gl_once_t; # define gl_once_define(STORAGECLASS, NAME) \ STORAGECLASS pth_once_t NAME = PTH_ONCE_INIT; # define glthread_once(ONCE_CONTROL, INITFUNCTION) \ (pth_in_use () \ ? glthread_once_multithreaded (ONCE_CONTROL, INITFUNCTION) \ : (glthread_once_singlethreaded (ONCE_CONTROL) ? (INITFUNCTION (), 0) : 0)) extern int glthread_once_multithreaded (pth_once_t *once_control, void (*initfunction) (void)); extern int glthread_once_singlethreaded (pth_once_t *once_control); # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_SOLARIS_THREADS /* Use the old Solaris threads library. */ # include # include # ifdef __cplusplus extern "C" { # endif # if USE_SOLARIS_THREADS_WEAK /* Use weak references to the old Solaris threads library. */ # pragma weak mutex_init # pragma weak mutex_lock # pragma weak mutex_unlock # pragma weak mutex_destroy # pragma weak rwlock_init # pragma weak rw_rdlock # pragma weak rw_wrlock # pragma weak rw_unlock # pragma weak rwlock_destroy # pragma weak thr_self # pragma weak thr_suspend # define thread_in_use() (thr_suspend != NULL) # else # define thread_in_use() 1 # endif /* -------------------------- gl_lock_t datatype -------------------------- */ typedef mutex_t gl_lock_t; # define gl_lock_define(STORAGECLASS, NAME) \ STORAGECLASS mutex_t NAME; # define gl_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS mutex_t NAME = gl_lock_initializer; # define gl_lock_initializer \ DEFAULTMUTEX # define glthread_lock_init(LOCK) \ (thread_in_use () ? mutex_init (LOCK, USYNC_THREAD, NULL) : 0) # define glthread_lock_lock(LOCK) \ (thread_in_use () ? mutex_lock (LOCK) : 0) # define glthread_lock_unlock(LOCK) \ (thread_in_use () ? mutex_unlock (LOCK) : 0) # define glthread_lock_destroy(LOCK) \ (thread_in_use () ? mutex_destroy (LOCK) : 0) /* ------------------------- gl_rwlock_t datatype ------------------------- */ typedef rwlock_t gl_rwlock_t; # define gl_rwlock_define(STORAGECLASS, NAME) \ STORAGECLASS rwlock_t NAME; # define gl_rwlock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS rwlock_t NAME = gl_rwlock_initializer; # define gl_rwlock_initializer \ DEFAULTRWLOCK # define glthread_rwlock_init(LOCK) \ (thread_in_use () ? rwlock_init (LOCK, USYNC_THREAD, NULL) : 0) # define glthread_rwlock_rdlock(LOCK) \ (thread_in_use () ? rw_rdlock (LOCK) : 0) # define glthread_rwlock_wrlock(LOCK) \ (thread_in_use () ? rw_wrlock (LOCK) : 0) # define glthread_rwlock_unlock(LOCK) \ (thread_in_use () ? rw_unlock (LOCK) : 0) # define glthread_rwlock_destroy(LOCK) \ (thread_in_use () ? rwlock_destroy (LOCK) : 0) /* --------------------- gl_recursive_lock_t datatype --------------------- */ /* Old Solaris threads did not have recursive locks. We have to implement them ourselves. */ typedef struct { mutex_t mutex; thread_t owner; unsigned long depth; } gl_recursive_lock_t; # define gl_recursive_lock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME; # define gl_recursive_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME = gl_recursive_lock_initializer; # define gl_recursive_lock_initializer \ { DEFAULTMUTEX, (thread_t) 0, 0 } # define glthread_recursive_lock_init(LOCK) \ (thread_in_use () ? glthread_recursive_lock_init_multithreaded (LOCK) : 0) # define glthread_recursive_lock_lock(LOCK) \ (thread_in_use () ? glthread_recursive_lock_lock_multithreaded (LOCK) : 0) # define glthread_recursive_lock_unlock(LOCK) \ (thread_in_use () ? glthread_recursive_lock_unlock_multithreaded (LOCK) : 0) # define glthread_recursive_lock_destroy(LOCK) \ (thread_in_use () ? glthread_recursive_lock_destroy_multithreaded (LOCK) : 0) extern int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_lock_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_unlock_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_destroy_multithreaded (gl_recursive_lock_t *lock); /* -------------------------- gl_once_t datatype -------------------------- */ typedef struct { volatile int inited; mutex_t mutex; } gl_once_t; # define gl_once_define(STORAGECLASS, NAME) \ STORAGECLASS gl_once_t NAME = { 0, DEFAULTMUTEX }; # define glthread_once(ONCE_CONTROL, INITFUNCTION) \ (thread_in_use () \ ? glthread_once_multithreaded (ONCE_CONTROL, INITFUNCTION) \ : (glthread_once_singlethreaded (ONCE_CONTROL) ? (INITFUNCTION (), 0) : 0)) extern int glthread_once_multithreaded (gl_once_t *once_control, void (*initfunction) (void)); extern int glthread_once_singlethreaded (gl_once_t *once_control); # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_WINDOWS_THREADS # define WIN32_LEAN_AND_MEAN /* avoid including junk */ # include # ifdef __cplusplus extern "C" { # endif /* We can use CRITICAL_SECTION directly, rather than the native Windows Event, Mutex, Semaphore types, because - we need only to synchronize inside a single process (address space), not inter-process locking, - we don't need to support trylock operations. (TryEnterCriticalSection does not work on Windows 95/98/ME. Packages that need trylock usually define their own mutex type.) */ /* There is no way to statically initialize a CRITICAL_SECTION. It needs to be done lazily, once only. For this we need spinlocks. */ typedef struct { volatile int done; volatile long started; } gl_spinlock_t; /* -------------------------- gl_lock_t datatype -------------------------- */ typedef struct { gl_spinlock_t guard; /* protects the initialization */ CRITICAL_SECTION lock; } gl_lock_t; # define gl_lock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_lock_t NAME; # define gl_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_lock_t NAME = gl_lock_initializer; # define gl_lock_initializer \ { { 0, -1 } } # define glthread_lock_init(LOCK) \ (glthread_lock_init_func (LOCK), 0) # define glthread_lock_lock(LOCK) \ glthread_lock_lock_func (LOCK) # define glthread_lock_unlock(LOCK) \ glthread_lock_unlock_func (LOCK) # define glthread_lock_destroy(LOCK) \ glthread_lock_destroy_func (LOCK) extern void glthread_lock_init_func (gl_lock_t *lock); extern int glthread_lock_lock_func (gl_lock_t *lock); extern int glthread_lock_unlock_func (gl_lock_t *lock); extern int glthread_lock_destroy_func (gl_lock_t *lock); /* ------------------------- gl_rwlock_t datatype ------------------------- */ /* It is impossible to implement read-write locks using plain locks, without introducing an extra thread dedicated to managing read-write locks. Therefore here we need to use the low-level Event type. */ typedef struct { HANDLE *array; /* array of waiting threads, each represented by an event */ unsigned int count; /* number of waiting threads */ unsigned int alloc; /* length of allocated array */ unsigned int offset; /* index of first waiting thread in array */ } gl_carray_waitqueue_t; typedef struct { gl_spinlock_t guard; /* protects the initialization */ CRITICAL_SECTION lock; /* protects the remaining fields */ gl_carray_waitqueue_t waiting_readers; /* waiting readers */ gl_carray_waitqueue_t waiting_writers; /* waiting writers */ int runcount; /* number of readers running, or -1 when a writer runs */ } gl_rwlock_t; # define gl_rwlock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_rwlock_t NAME; # define gl_rwlock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_rwlock_t NAME = gl_rwlock_initializer; # define gl_rwlock_initializer \ { { 0, -1 } } # define glthread_rwlock_init(LOCK) \ (glthread_rwlock_init_func (LOCK), 0) # define glthread_rwlock_rdlock(LOCK) \ glthread_rwlock_rdlock_func (LOCK) # define glthread_rwlock_wrlock(LOCK) \ glthread_rwlock_wrlock_func (LOCK) # define glthread_rwlock_unlock(LOCK) \ glthread_rwlock_unlock_func (LOCK) # define glthread_rwlock_destroy(LOCK) \ glthread_rwlock_destroy_func (LOCK) extern void glthread_rwlock_init_func (gl_rwlock_t *lock); extern int glthread_rwlock_rdlock_func (gl_rwlock_t *lock); extern int glthread_rwlock_wrlock_func (gl_rwlock_t *lock); extern int glthread_rwlock_unlock_func (gl_rwlock_t *lock); extern int glthread_rwlock_destroy_func (gl_rwlock_t *lock); /* --------------------- gl_recursive_lock_t datatype --------------------- */ /* The native Windows documentation says that CRITICAL_SECTION already implements a recursive lock. But we need not rely on it: It's easy to implement a recursive lock without this assumption. */ typedef struct { gl_spinlock_t guard; /* protects the initialization */ DWORD owner; unsigned long depth; CRITICAL_SECTION lock; } gl_recursive_lock_t; # define gl_recursive_lock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME; # define gl_recursive_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME = gl_recursive_lock_initializer; # define gl_recursive_lock_initializer \ { { 0, -1 }, 0, 0 } # define glthread_recursive_lock_init(LOCK) \ (glthread_recursive_lock_init_func (LOCK), 0) # define glthread_recursive_lock_lock(LOCK) \ glthread_recursive_lock_lock_func (LOCK) # define glthread_recursive_lock_unlock(LOCK) \ glthread_recursive_lock_unlock_func (LOCK) # define glthread_recursive_lock_destroy(LOCK) \ glthread_recursive_lock_destroy_func (LOCK) extern void glthread_recursive_lock_init_func (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_lock_func (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_unlock_func (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_destroy_func (gl_recursive_lock_t *lock); /* -------------------------- gl_once_t datatype -------------------------- */ typedef struct { volatile int inited; volatile long started; CRITICAL_SECTION lock; } gl_once_t; # define gl_once_define(STORAGECLASS, NAME) \ STORAGECLASS gl_once_t NAME = { -1, -1 }; # define glthread_once(ONCE_CONTROL, INITFUNCTION) \ (glthread_once_func (ONCE_CONTROL, INITFUNCTION), 0) extern void glthread_once_func (gl_once_t *once_control, void (*initfunction) (void)); # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if !(USE_POSIX_THREADS || USE_PTH_THREADS || USE_SOLARIS_THREADS || USE_WINDOWS_THREADS) /* Provide dummy implementation if threads are not supported. */ /* -------------------------- gl_lock_t datatype -------------------------- */ typedef int gl_lock_t; # define gl_lock_define(STORAGECLASS, NAME) # define gl_lock_define_initialized(STORAGECLASS, NAME) # define glthread_lock_init(NAME) 0 # define glthread_lock_lock(NAME) 0 # define glthread_lock_unlock(NAME) 0 # define glthread_lock_destroy(NAME) 0 /* ------------------------- gl_rwlock_t datatype ------------------------- */ typedef int gl_rwlock_t; # define gl_rwlock_define(STORAGECLASS, NAME) # define gl_rwlock_define_initialized(STORAGECLASS, NAME) # define glthread_rwlock_init(NAME) 0 # define glthread_rwlock_rdlock(NAME) 0 # define glthread_rwlock_wrlock(NAME) 0 # define glthread_rwlock_unlock(NAME) 0 # define glthread_rwlock_destroy(NAME) 0 /* --------------------- gl_recursive_lock_t datatype --------------------- */ typedef int gl_recursive_lock_t; # define gl_recursive_lock_define(STORAGECLASS, NAME) # define gl_recursive_lock_define_initialized(STORAGECLASS, NAME) # define glthread_recursive_lock_init(NAME) 0 # define glthread_recursive_lock_lock(NAME) 0 # define glthread_recursive_lock_unlock(NAME) 0 # define glthread_recursive_lock_destroy(NAME) 0 /* -------------------------- gl_once_t datatype -------------------------- */ typedef int gl_once_t; # define gl_once_define(STORAGECLASS, NAME) \ STORAGECLASS gl_once_t NAME = 0; # define glthread_once(ONCE_CONTROL, INITFUNCTION) \ (*(ONCE_CONTROL) == 0 ? (*(ONCE_CONTROL) = ~ 0, INITFUNCTION (), 0) : 0) #endif /* ========================================================================= */ /* Macros with built-in error handling. */ /* -------------------------- gl_lock_t datatype -------------------------- */ #define gl_lock_init(NAME) \ do \ { \ if (glthread_lock_init (&NAME)) \ abort (); \ } \ while (0) #define gl_lock_lock(NAME) \ do \ { \ if (glthread_lock_lock (&NAME)) \ abort (); \ } \ while (0) #define gl_lock_unlock(NAME) \ do \ { \ if (glthread_lock_unlock (&NAME)) \ abort (); \ } \ while (0) #define gl_lock_destroy(NAME) \ do \ { \ if (glthread_lock_destroy (&NAME)) \ abort (); \ } \ while (0) /* ------------------------- gl_rwlock_t datatype ------------------------- */ #define gl_rwlock_init(NAME) \ do \ { \ if (glthread_rwlock_init (&NAME)) \ abort (); \ } \ while (0) #define gl_rwlock_rdlock(NAME) \ do \ { \ if (glthread_rwlock_rdlock (&NAME)) \ abort (); \ } \ while (0) #define gl_rwlock_wrlock(NAME) \ do \ { \ if (glthread_rwlock_wrlock (&NAME)) \ abort (); \ } \ while (0) #define gl_rwlock_unlock(NAME) \ do \ { \ if (glthread_rwlock_unlock (&NAME)) \ abort (); \ } \ while (0) #define gl_rwlock_destroy(NAME) \ do \ { \ if (glthread_rwlock_destroy (&NAME)) \ abort (); \ } \ while (0) /* --------------------- gl_recursive_lock_t datatype --------------------- */ #define gl_recursive_lock_init(NAME) \ do \ { \ if (glthread_recursive_lock_init (&NAME)) \ abort (); \ } \ while (0) #define gl_recursive_lock_lock(NAME) \ do \ { \ if (glthread_recursive_lock_lock (&NAME)) \ abort (); \ } \ while (0) #define gl_recursive_lock_unlock(NAME) \ do \ { \ if (glthread_recursive_lock_unlock (&NAME)) \ abort (); \ } \ while (0) #define gl_recursive_lock_destroy(NAME) \ do \ { \ if (glthread_recursive_lock_destroy (&NAME)) \ abort (); \ } \ while (0) /* -------------------------- gl_once_t datatype -------------------------- */ #define gl_once(NAME, INITFUNCTION) \ do \ { \ if (glthread_once (&NAME, INITFUNCTION)) \ abort (); \ } \ while (0) /* ========================================================================= */ #endif /* _LOCK_H */ gnuastro-0.2.33-8a3b/bootstrapped/README0000644000175000017500000000251712722534072014514 00000000000000Imported files to GNU Astronomy Utilities ========================================= The contents of this directory (except this README file!) are imported to GNU Astronomy Utilities (Gnuastro) from other projects. Therefore they are not maintained by Gnuastro developers and separately kept in this directory for clarity and easy maintainence. In the version controlled repository this directory only contains this single README file. It is populated during the bootstrapping process (see ../README-hacking for more on bootstrapping, or the "Bootstrapping" section in the manual). In the distribution tar-ball this directory is populated with the relevant necessary files. The projects that were used are: - GNU Portability Library (Gnulib): https://www.gnu.org/software/gnulib/ This is a very useful collection of libraries (from GNU C library) to enable non-complying operating systems to run programs based on it. It also contains various very useful scripts needed for the GNU build process. - GNU Autoconf-archives: https://www.gnu.org/software/autoconf-archive/ These archives contain a large number of M4 scripts that can be used at ./configure time. We are most grateful to the maintainers of these projects which allow Gnuastro to be easily installed on a very large set of Unix-like operating systems.gnuastro-0.2.33-8a3b/bootstrapped/m4/0000755000175000017500000000000013004464723014226 500000000000000gnuastro-0.2.33-8a3b/bootstrapped/m4/gnulib-cache.m40000644000175000017500000000413613004436760016735 00000000000000# Copyright (C) 2002-2016 Free Software Foundation, Inc. # # This file is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This file is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this file. If not, see . # # As a special exception to the GNU General Public License, # this file may be distributed as part of a program that # contains a configuration script generated by Autoconf, under # the same distribution terms as the rest of that program. # # Generated by gnulib-tool. # # This file represents the specification of how gnulib-tool is used. # It acts as a cache: It is written and read by gnulib-tool. # In projects that use version control, this file is meant to be put under # version control, like the configure.ac and various Makefile.am files. # Specification in the form of a command-line invocation: # gnulib-tool --import --local-dir=gl --lib=libgnu --source-base=bootstrapped/lib --m4-base=bootstrapped/m4 --doc-base=bootstrapped/doc --tests-base=bootstrapped/tests --aux-dir=bootstrapped/build-aux --with-tests --no-conditional-dependencies --libtool --macro-prefix=gl --no-vc-files argp error fdl gendocs git-version-gen math nproc regex strcase # Specification in the form of a few gnulib-tool.m4 macro invocations: gl_LOCAL_DIR([gl]) gl_MODULES([ argp error fdl gendocs git-version-gen math nproc regex strcase ]) gl_AVOID([]) gl_SOURCE_BASE([bootstrapped/lib]) gl_M4_BASE([bootstrapped/m4]) gl_PO_BASE([]) gl_DOC_BASE([bootstrapped/doc]) gl_TESTS_BASE([bootstrapped/tests]) gl_WITH_TESTS gl_LIB([libgnu]) gl_MAKEFILE_NAME([]) gl_LIBTOOL gl_MACRO_PREFIX([gl]) gl_PO_DOMAIN([]) gl_WITNESS_C_MACRO([]) gl_VC_FILES([false]) gnuastro-0.2.33-8a3b/bootstrapped/m4/yield.m40000644000175000017500000000135713004436755015530 00000000000000# yield.m4 serial 2 dnl Copyright (C) 2005-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_YIELD], [ AC_REQUIRE([gl_THREADLIB]) dnl On some systems, sched_yield is in librt, rather than in libpthread. YIELD_LIB= if test $gl_threads_api = posix; then dnl Solaris has sched_yield in librt, not in libpthread or libc. AC_CHECK_LIB([rt], [sched_yield], [YIELD_LIB=-lrt], [dnl Solaris 2.5.1, 2.6 has sched_yield in libposix4, not librt. AC_CHECK_LIB([posix4], [sched_yield], [YIELD_LIB=-lposix4])]) fi AC_SUBST([YIELD_LIB]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/xsize.m40000644000175000017500000000062613004436755015562 00000000000000# xsize.m4 serial 5 dnl Copyright (C) 2003-2004, 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_XSIZE], [ dnl Prerequisites of lib/xsize.h. AC_REQUIRE([gl_SIZE_MAX]) AC_CHECK_HEADERS([stdint.h]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/wint_t.m40000644000175000017500000000203513004436755015720 00000000000000# wint_t.m4 serial 5 (gettext-0.18.2) dnl Copyright (C) 2003, 2007-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl Test whether has the 'wint_t' type. dnl Prerequisite: AC_PROG_CC AC_DEFUN([gt_TYPE_WINT_T], [ AC_CACHE_CHECK([for wint_t], [gt_cv_c_wint_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include wint_t foo = (wchar_t)'\0';]], [[]])], [gt_cv_c_wint_t=yes], [gt_cv_c_wint_t=no])]) if test $gt_cv_c_wint_t = yes; then AC_DEFINE([HAVE_WINT_T], [1], [Define if you have the 'wint_t' type.]) fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/wctype_h.m40000644000175000017500000001543513004436755016246 00000000000000# wctype_h.m4 serial 18 dnl A placeholder for ISO C99 , for platforms that lack it. dnl Copyright (C) 2006-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Written by Paul Eggert. AC_DEFUN([gl_WCTYPE_H], [ AC_REQUIRE([gl_WCTYPE_H_DEFAULTS]) AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) AC_CHECK_FUNCS_ONCE([iswcntrl]) if test $ac_cv_func_iswcntrl = yes; then HAVE_ISWCNTRL=1 else HAVE_ISWCNTRL=0 fi AC_SUBST([HAVE_ISWCNTRL]) AC_REQUIRE([gt_TYPE_WINT_T]) if test $gt_cv_c_wint_t = yes; then HAVE_WINT_T=1 else HAVE_WINT_T=0 fi AC_SUBST([HAVE_WINT_T]) gl_CHECK_NEXT_HEADERS([wctype.h]) if test $ac_cv_header_wctype_h = yes; then if test $ac_cv_func_iswcntrl = yes; then dnl Linux libc5 has an iswprint function that returns 0 for all arguments. dnl The other functions are likely broken in the same way. AC_CACHE_CHECK([whether iswcntrl works], [gl_cv_func_iswcntrl_works], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #include int main () { return iswprint ('x') == 0; } ]])], [gl_cv_func_iswcntrl_works=yes], [gl_cv_func_iswcntrl_works=no], [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[#include #if __GNU_LIBRARY__ == 1 Linux libc5 i18n is broken. #endif]], [])], [gl_cv_func_iswcntrl_works="guessing yes"], [gl_cv_func_iswcntrl_works="guessing no"]) ]) ]) fi HAVE_WCTYPE_H=1 else HAVE_WCTYPE_H=0 fi AC_SUBST([HAVE_WCTYPE_H]) case "$gl_cv_func_iswcntrl_works" in *yes) REPLACE_ISWCNTRL=0 ;; *) REPLACE_ISWCNTRL=1 ;; esac AC_SUBST([REPLACE_ISWCNTRL]) if test $HAVE_ISWCNTRL = 0 || test $REPLACE_ISWCNTRL = 1; then dnl Redefine all of iswcntrl, ..., iswxdigit in . : fi if test $REPLACE_ISWCNTRL = 1; then REPLACE_TOWLOWER=1 else AC_CHECK_FUNCS([towlower]) if test $ac_cv_func_towlower = yes; then REPLACE_TOWLOWER=0 else AC_CHECK_DECLS([towlower],,, [[/* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #if HAVE_WCTYPE_H # include #endif ]]) if test $ac_cv_have_decl_towlower = yes; then dnl On Minix 3.1.8, the system's declares towlower() and dnl towupper() although it does not have the functions. Avoid a dnl collision with gnulib's replacement. REPLACE_TOWLOWER=1 else REPLACE_TOWLOWER=0 fi fi fi AC_SUBST([REPLACE_TOWLOWER]) if test $HAVE_ISWCNTRL = 0 || test $REPLACE_TOWLOWER = 1; then dnl Redefine towlower, towupper in . : fi dnl We assume that the wctype() and iswctype() functions exist if and only dnl if the type wctype_t is defined in or in if that dnl exists. dnl HP-UX 11.00 declares all these in and lacks . AC_CACHE_CHECK([for wctype_t], [gl_cv_type_wctype_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[/* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #if HAVE_WCTYPE_H # include #endif wctype_t a; ]], [[]])], [gl_cv_type_wctype_t=yes], [gl_cv_type_wctype_t=no]) ]) if test $gl_cv_type_wctype_t = no; then HAVE_WCTYPE_T=0 fi dnl We assume that the wctrans() and towctrans() functions exist if and only dnl if the type wctrans_t is defined in . AC_CACHE_CHECK([for wctrans_t], [gl_cv_type_wctrans_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[/* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #include wctrans_t a; ]], [[]])], [gl_cv_type_wctrans_t=yes], [gl_cv_type_wctrans_t=no]) ]) if test $gl_cv_type_wctrans_t = no; then HAVE_WCTRANS_T=0 fi dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include # include # include # include #endif #include ]], [wctype iswctype wctrans towctrans ]) ]) AC_DEFUN([gl_WCTYPE_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_WCTYPE_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_WCTYPE_H_DEFAULTS], [ GNULIB_ISWBLANK=0; AC_SUBST([GNULIB_ISWBLANK]) GNULIB_WCTYPE=0; AC_SUBST([GNULIB_WCTYPE]) GNULIB_ISWCTYPE=0; AC_SUBST([GNULIB_ISWCTYPE]) GNULIB_WCTRANS=0; AC_SUBST([GNULIB_WCTRANS]) GNULIB_TOWCTRANS=0; AC_SUBST([GNULIB_TOWCTRANS]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_ISWBLANK=1; AC_SUBST([HAVE_ISWBLANK]) HAVE_WCTYPE_T=1; AC_SUBST([HAVE_WCTYPE_T]) HAVE_WCTRANS_T=1; AC_SUBST([HAVE_WCTRANS_T]) REPLACE_ISWBLANK=0; AC_SUBST([REPLACE_ISWBLANK]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/wctomb.m40000644000175000017500000000071413004436755015711 00000000000000# wctomb.m4 serial 2 dnl Copyright (C) 2011-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_WCTOMB], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) if false; then REPLACE_WCTOMB=1 fi ]) # Prerequisites of lib/wctomb.c. AC_DEFUN([gl_PREREQ_WCTOMB], [ : ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/wctob.m40000644000175000017500000000667613004436755015551 00000000000000# wctob.m4 serial 10 dnl Copyright (C) 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_WCTOB], [ AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) AC_CHECK_FUNCS_ONCE([wctob]) if test $ac_cv_func_wctob = no; then HAVE_WCTOB=0 HAVE_DECL_WCTOB=0 else HAVE_WCTOB=1 dnl Solaris 9 has the wctob() function but it does not work. dnl Cygwin 1.7.2 has the wctob() function but it clobbers caller-owned dnl registers, see . AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_FR]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether wctob works], [gl_cv_func_wctob_works], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on Solaris <= 9 and Cygwin. solaris2.[1-9] | solaris2.[1-9].* | cygwin*) gl_cv_func_wctob_works="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_wctob_works="guessing yes" ;; esac changequote([,])dnl case "$host_os" in cygwin*) AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include register long global __asm__ ("%ebx"); int main () { setlocale (LC_ALL, "en_US.UTF-8"); global = 0x12345678; if (wctob (0x00FC) != -1) return 1; if (global != 0x12345678) return 2; return 0; }]])], [:], [gl_cv_func_wctob_works=no], [:]) ;; esac if test "$gl_cv_func_wctob_works" != no && test $LOCALE_FR != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_FR") != NULL) { wchar_t wc; if (mbtowc (&wc, "\374", 1) == 1) if (wctob (wc) != (unsigned char) '\374') return 1; } return 0; }]])], [gl_cv_func_wctob_works=yes], [gl_cv_func_wctob_works=no], [:]) fi ]) case "$gl_cv_func_wctob_works" in *yes) ;; *) REPLACE_WCTOB=1 ;; esac if test $REPLACE_WCTOB = 0; then dnl IRIX 6.5 has the wctob() function but does not declare it. AC_CHECK_DECLS([wctob], [], [], [[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include ]]) if test $ac_cv_have_decl_wctob != yes; then HAVE_DECL_WCTOB=0 fi fi fi ]) # Prerequisites of lib/wctob.c. AC_DEFUN([gl_PREREQ_WCTOB], [ : ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/wcrtomb.m40000644000175000017500000000661013004436755016074 00000000000000# wcrtomb.m4 serial 11 dnl Copyright (C) 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_WCRTOMB], [ AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) AC_REQUIRE([AC_TYPE_MBSTATE_T]) gl_MBSTATE_T_BROKEN AC_CHECK_FUNCS_ONCE([wcrtomb]) if test $ac_cv_func_wcrtomb = no; then HAVE_WCRTOMB=0 AC_CHECK_DECLS([wcrtomb],,, [[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include ]]) if test $ac_cv_have_decl_wcrtomb = yes; then dnl On Minix 3.1.8, the system's declares wcrtomb() although dnl it does not have the function. Avoid a collision with gnulib's dnl replacement. REPLACE_WCRTOMB=1 fi else if test $REPLACE_MBSTATE_T = 1; then REPLACE_WCRTOMB=1 else dnl On AIX 4.3, OSF/1 5.1 and Solaris 10, wcrtomb (NULL, 0, NULL) sometimes dnl returns 0 instead of 1. AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_FR]) AC_REQUIRE([gt_LOCALE_FR_UTF8]) AC_REQUIRE([gt_LOCALE_JA]) AC_REQUIRE([gt_LOCALE_ZH_CN]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether wcrtomb return value is correct], [gl_cv_func_wcrtomb_retval], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on AIX 4, OSF/1 and Solaris. aix4* | osf* | solaris*) gl_cv_func_wcrtomb_retval="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_wcrtomb_retval="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_FR != none || test $LOCALE_FR_UTF8 != none || test $LOCALE_JA != none || test $LOCALE_ZH_CN != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { int result = 0; if (setlocale (LC_ALL, "$LOCALE_FR") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 1; } if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 2; } if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 4; } if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 8; } return result; }]])], [gl_cv_func_wcrtomb_retval=yes], [gl_cv_func_wcrtomb_retval=no], [:]) fi ]) case "$gl_cv_func_wcrtomb_retval" in *yes) ;; *) REPLACE_WCRTOMB=1 ;; esac fi fi ]) # Prerequisites of lib/wcrtomb.c. AC_DEFUN([gl_PREREQ_WCRTOMB], [ : ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/wchar_t.m40000644000175000017500000000146213004436755016046 00000000000000# wchar_t.m4 serial 4 (gettext-0.18.2) dnl Copyright (C) 2002-2003, 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl Test whether has the 'wchar_t' type. dnl Prerequisite: AC_PROG_CC AC_DEFUN([gt_TYPE_WCHAR_T], [ AC_CACHE_CHECK([for wchar_t], [gt_cv_c_wchar_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include wchar_t foo = (wchar_t)'\0';]], [[]])], [gt_cv_c_wchar_t=yes], [gt_cv_c_wchar_t=no])]) if test $gt_cv_c_wchar_t = yes; then AC_DEFINE([HAVE_WCHAR_T], [1], [Define if you have the 'wchar_t' type.]) fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/wchar_h.m40000644000175000017500000002322613004436755016034 00000000000000dnl A placeholder for ISO C99 , for platforms that have issues. dnl Copyright (C) 2007-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Written by Eric Blake. # wchar_h.m4 serial 40 AC_DEFUN([gl_WCHAR_H], [ AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) AC_REQUIRE([gl_WCHAR_H_INLINE_OK]) dnl Prepare for creating substitute . dnl Check for (missing in Linux uClibc when built without wide dnl character support). dnl is always overridden, because of GNULIB_POSIXCHECK. gl_CHECK_NEXT_HEADERS([wchar.h]) if test $ac_cv_header_wchar_h = yes; then HAVE_WCHAR_H=1 else HAVE_WCHAR_H=0 fi AC_SUBST([HAVE_WCHAR_H]) AC_REQUIRE([gl_FEATURES_H]) AC_REQUIRE([gt_TYPE_WINT_T]) if test $gt_cv_c_wint_t = yes; then HAVE_WINT_T=1 else HAVE_WINT_T=0 fi AC_SUBST([HAVE_WINT_T]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include # include # include #endif #include ]], [btowc wctob mbsinit mbrtowc mbrlen mbsrtowcs mbsnrtowcs wcrtomb wcsrtombs wcsnrtombs wcwidth wmemchr wmemcmp wmemcpy wmemmove wmemset wcslen wcsnlen wcscpy wcpcpy wcsncpy wcpncpy wcscat wcsncat wcscmp wcsncmp wcscasecmp wcsncasecmp wcscoll wcsxfrm wcsdup wcschr wcsrchr wcscspn wcsspn wcspbrk wcsstr wcstok wcswidth ]) ]) dnl Check whether is usable at all. AC_DEFUN([gl_WCHAR_H_INLINE_OK], [ dnl Test whether suffers due to the transition from '__inline' to dnl 'gnu_inline'. See dnl and . In summary, dnl glibc version 2.5 or older, together with gcc version 4.3 or newer and dnl the option -std=c99 or -std=gnu99, leads to a broken . AC_CACHE_CHECK([whether uses 'inline' correctly], [gl_cv_header_wchar_h_correct_inline], [gl_cv_header_wchar_h_correct_inline=yes AC_LANG_CONFTEST([ AC_LANG_SOURCE([[#define wcstod renamed_wcstod /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include extern int zero (void); int main () { return zero(); } ]])]) dnl Do not rename the object file from conftest.$ac_objext to dnl conftest1.$ac_objext, as this will cause the link to fail on dnl z/OS when using the XPLINK object format (due to duplicate dnl CSECT names). Instead, temporarily redefine $ac_compile so dnl that the object file has the latter name from the start. save_ac_compile="$ac_compile" ac_compile=`echo "$save_ac_compile" | sed s/conftest/conftest1/` if AC_TRY_EVAL([ac_compile]); then AC_LANG_CONFTEST([ AC_LANG_SOURCE([[#define wcstod renamed_wcstod /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int zero (void) { return 0; } ]])]) dnl See note above about renaming object files. ac_compile=`echo "$save_ac_compile" | sed s/conftest/conftest2/` if AC_TRY_EVAL([ac_compile]); then if $CC -o conftest$ac_exeext $CFLAGS $LDFLAGS conftest1.$ac_objext conftest2.$ac_objext $LIBS >&AS_MESSAGE_LOG_FD 2>&1; then : else gl_cv_header_wchar_h_correct_inline=no fi fi fi ac_compile="$save_ac_compile" rm -f conftest1.$ac_objext conftest2.$ac_objext conftest$ac_exeext ]) if test $gl_cv_header_wchar_h_correct_inline = no; then AC_MSG_ERROR([ cannot be used with this compiler ($CC $CFLAGS $CPPFLAGS). This is a known interoperability problem of glibc <= 2.5 with gcc >= 4.3 in C99 mode. You have four options: - Add the flag -fgnu89-inline to CC and reconfigure, or - Fix your include files, using parts of , or - Use a gcc version older than 4.3, or - Don't use the flags -std=c99 or -std=gnu99. Configuration aborted.]) fi ]) AC_DEFUN([gl_WCHAR_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_WCHAR_H_DEFAULTS], [ GNULIB_BTOWC=0; AC_SUBST([GNULIB_BTOWC]) GNULIB_WCTOB=0; AC_SUBST([GNULIB_WCTOB]) GNULIB_MBSINIT=0; AC_SUBST([GNULIB_MBSINIT]) GNULIB_MBRTOWC=0; AC_SUBST([GNULIB_MBRTOWC]) GNULIB_MBRLEN=0; AC_SUBST([GNULIB_MBRLEN]) GNULIB_MBSRTOWCS=0; AC_SUBST([GNULIB_MBSRTOWCS]) GNULIB_MBSNRTOWCS=0; AC_SUBST([GNULIB_MBSNRTOWCS]) GNULIB_WCRTOMB=0; AC_SUBST([GNULIB_WCRTOMB]) GNULIB_WCSRTOMBS=0; AC_SUBST([GNULIB_WCSRTOMBS]) GNULIB_WCSNRTOMBS=0; AC_SUBST([GNULIB_WCSNRTOMBS]) GNULIB_WCWIDTH=0; AC_SUBST([GNULIB_WCWIDTH]) GNULIB_WMEMCHR=0; AC_SUBST([GNULIB_WMEMCHR]) GNULIB_WMEMCMP=0; AC_SUBST([GNULIB_WMEMCMP]) GNULIB_WMEMCPY=0; AC_SUBST([GNULIB_WMEMCPY]) GNULIB_WMEMMOVE=0; AC_SUBST([GNULIB_WMEMMOVE]) GNULIB_WMEMSET=0; AC_SUBST([GNULIB_WMEMSET]) GNULIB_WCSLEN=0; AC_SUBST([GNULIB_WCSLEN]) GNULIB_WCSNLEN=0; AC_SUBST([GNULIB_WCSNLEN]) GNULIB_WCSCPY=0; AC_SUBST([GNULIB_WCSCPY]) GNULIB_WCPCPY=0; AC_SUBST([GNULIB_WCPCPY]) GNULIB_WCSNCPY=0; AC_SUBST([GNULIB_WCSNCPY]) GNULIB_WCPNCPY=0; AC_SUBST([GNULIB_WCPNCPY]) GNULIB_WCSCAT=0; AC_SUBST([GNULIB_WCSCAT]) GNULIB_WCSNCAT=0; AC_SUBST([GNULIB_WCSNCAT]) GNULIB_WCSCMP=0; AC_SUBST([GNULIB_WCSCMP]) GNULIB_WCSNCMP=0; AC_SUBST([GNULIB_WCSNCMP]) GNULIB_WCSCASECMP=0; AC_SUBST([GNULIB_WCSCASECMP]) GNULIB_WCSNCASECMP=0; AC_SUBST([GNULIB_WCSNCASECMP]) GNULIB_WCSCOLL=0; AC_SUBST([GNULIB_WCSCOLL]) GNULIB_WCSXFRM=0; AC_SUBST([GNULIB_WCSXFRM]) GNULIB_WCSDUP=0; AC_SUBST([GNULIB_WCSDUP]) GNULIB_WCSCHR=0; AC_SUBST([GNULIB_WCSCHR]) GNULIB_WCSRCHR=0; AC_SUBST([GNULIB_WCSRCHR]) GNULIB_WCSCSPN=0; AC_SUBST([GNULIB_WCSCSPN]) GNULIB_WCSSPN=0; AC_SUBST([GNULIB_WCSSPN]) GNULIB_WCSPBRK=0; AC_SUBST([GNULIB_WCSPBRK]) GNULIB_WCSSTR=0; AC_SUBST([GNULIB_WCSSTR]) GNULIB_WCSTOK=0; AC_SUBST([GNULIB_WCSTOK]) GNULIB_WCSWIDTH=0; AC_SUBST([GNULIB_WCSWIDTH]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_BTOWC=1; AC_SUBST([HAVE_BTOWC]) HAVE_MBSINIT=1; AC_SUBST([HAVE_MBSINIT]) HAVE_MBRTOWC=1; AC_SUBST([HAVE_MBRTOWC]) HAVE_MBRLEN=1; AC_SUBST([HAVE_MBRLEN]) HAVE_MBSRTOWCS=1; AC_SUBST([HAVE_MBSRTOWCS]) HAVE_MBSNRTOWCS=1; AC_SUBST([HAVE_MBSNRTOWCS]) HAVE_WCRTOMB=1; AC_SUBST([HAVE_WCRTOMB]) HAVE_WCSRTOMBS=1; AC_SUBST([HAVE_WCSRTOMBS]) HAVE_WCSNRTOMBS=1; AC_SUBST([HAVE_WCSNRTOMBS]) HAVE_WMEMCHR=1; AC_SUBST([HAVE_WMEMCHR]) HAVE_WMEMCMP=1; AC_SUBST([HAVE_WMEMCMP]) HAVE_WMEMCPY=1; AC_SUBST([HAVE_WMEMCPY]) HAVE_WMEMMOVE=1; AC_SUBST([HAVE_WMEMMOVE]) HAVE_WMEMSET=1; AC_SUBST([HAVE_WMEMSET]) HAVE_WCSLEN=1; AC_SUBST([HAVE_WCSLEN]) HAVE_WCSNLEN=1; AC_SUBST([HAVE_WCSNLEN]) HAVE_WCSCPY=1; AC_SUBST([HAVE_WCSCPY]) HAVE_WCPCPY=1; AC_SUBST([HAVE_WCPCPY]) HAVE_WCSNCPY=1; AC_SUBST([HAVE_WCSNCPY]) HAVE_WCPNCPY=1; AC_SUBST([HAVE_WCPNCPY]) HAVE_WCSCAT=1; AC_SUBST([HAVE_WCSCAT]) HAVE_WCSNCAT=1; AC_SUBST([HAVE_WCSNCAT]) HAVE_WCSCMP=1; AC_SUBST([HAVE_WCSCMP]) HAVE_WCSNCMP=1; AC_SUBST([HAVE_WCSNCMP]) HAVE_WCSCASECMP=1; AC_SUBST([HAVE_WCSCASECMP]) HAVE_WCSNCASECMP=1; AC_SUBST([HAVE_WCSNCASECMP]) HAVE_WCSCOLL=1; AC_SUBST([HAVE_WCSCOLL]) HAVE_WCSXFRM=1; AC_SUBST([HAVE_WCSXFRM]) HAVE_WCSDUP=1; AC_SUBST([HAVE_WCSDUP]) HAVE_WCSCHR=1; AC_SUBST([HAVE_WCSCHR]) HAVE_WCSRCHR=1; AC_SUBST([HAVE_WCSRCHR]) HAVE_WCSCSPN=1; AC_SUBST([HAVE_WCSCSPN]) HAVE_WCSSPN=1; AC_SUBST([HAVE_WCSSPN]) HAVE_WCSPBRK=1; AC_SUBST([HAVE_WCSPBRK]) HAVE_WCSSTR=1; AC_SUBST([HAVE_WCSSTR]) HAVE_WCSTOK=1; AC_SUBST([HAVE_WCSTOK]) HAVE_WCSWIDTH=1; AC_SUBST([HAVE_WCSWIDTH]) HAVE_DECL_WCTOB=1; AC_SUBST([HAVE_DECL_WCTOB]) HAVE_DECL_WCWIDTH=1; AC_SUBST([HAVE_DECL_WCWIDTH]) REPLACE_MBSTATE_T=0; AC_SUBST([REPLACE_MBSTATE_T]) REPLACE_BTOWC=0; AC_SUBST([REPLACE_BTOWC]) REPLACE_WCTOB=0; AC_SUBST([REPLACE_WCTOB]) REPLACE_MBSINIT=0; AC_SUBST([REPLACE_MBSINIT]) REPLACE_MBRTOWC=0; AC_SUBST([REPLACE_MBRTOWC]) REPLACE_MBRLEN=0; AC_SUBST([REPLACE_MBRLEN]) REPLACE_MBSRTOWCS=0; AC_SUBST([REPLACE_MBSRTOWCS]) REPLACE_MBSNRTOWCS=0; AC_SUBST([REPLACE_MBSNRTOWCS]) REPLACE_WCRTOMB=0; AC_SUBST([REPLACE_WCRTOMB]) REPLACE_WCSRTOMBS=0; AC_SUBST([REPLACE_WCSRTOMBS]) REPLACE_WCSNRTOMBS=0; AC_SUBST([REPLACE_WCSNRTOMBS]) REPLACE_WCWIDTH=0; AC_SUBST([REPLACE_WCWIDTH]) REPLACE_WCSWIDTH=0; AC_SUBST([REPLACE_WCSWIDTH]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/warn-on-use.m40000644000175000017500000000415413004436755016573 00000000000000# warn-on-use.m4 serial 5 dnl Copyright (C) 2010-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # gl_WARN_ON_USE_PREPARE(INCLUDES, NAMES) # --------------------------------------- # For each whitespace-separated element in the list of NAMES, define # HAVE_RAW_DECL_name if the function has a declaration among INCLUDES # even after being undefined as a macro. # # See warn-on-use.h for some hints on how to poison function names, as # well as ideas on poisoning global variables and macros. NAMES may # include global variables, but remember that only functions work with # _GL_WARN_ON_USE. Typically, INCLUDES only needs to list a single # header, but if the replacement header pulls in other headers because # some systems declare functions in the wrong header, then INCLUDES # should do likewise. # # It is generally safe to assume declarations for functions declared # in the intersection of C89 and C11 (such as printf) without # needing gl_WARN_ON_USE_PREPARE. AC_DEFUN([gl_WARN_ON_USE_PREPARE], [ m4_foreach_w([gl_decl], [$2], [AH_TEMPLATE([HAVE_RAW_DECL_]AS_TR_CPP(m4_defn([gl_decl])), [Define to 1 if ]m4_defn([gl_decl])[ is declared even after undefining macros.])])dnl dnl FIXME: gl_Symbol must be used unquoted until we can assume dnl autoconf 2.64 or newer. for gl_func in m4_flatten([$2]); do AS_VAR_PUSHDEF([gl_Symbol], [gl_cv_have_raw_decl_$gl_func])dnl AC_CACHE_CHECK([whether $gl_func is declared without a macro], gl_Symbol, [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([$1], [@%:@undef $gl_func (void) $gl_func;])], [AS_VAR_SET(gl_Symbol, [yes])], [AS_VAR_SET(gl_Symbol, [no])])]) AS_VAR_IF(gl_Symbol, [yes], [AC_DEFINE_UNQUOTED(AS_TR_CPP([HAVE_RAW_DECL_$gl_func]), [1]) dnl shortcut - if the raw declaration exists, then set a cache dnl variable to allow skipping any later AC_CHECK_DECL efforts eval ac_cv_have_decl_$gl_func=yes]) AS_VAR_POPDEF([gl_Symbol])dnl done ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/vsnprintf.m40000644000175000017500000000310213004436755016441 00000000000000# vsnprintf.m4 serial 6 dnl Copyright (C) 2002-2004, 2007-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Libintl 0.17 will replace vsnprintf only if it does not support %1$s, dnl but defers to any gnulib vsnprintf replacements. Therefore, gnulib dnl must guarantee that the decision for replacing vsnprintf is a superset dnl of the reasons checked by libintl. AC_DEFUN([gl_FUNC_VSNPRINTF], [ AC_REQUIRE([gl_STDIO_H_DEFAULTS]) gl_cv_func_vsnprintf_usable=no AC_CHECK_FUNCS([vsnprintf]) if test $ac_cv_func_vsnprintf = yes; then gl_SNPRINTF_SIZE1 case "$gl_cv_func_snprintf_size1" in *yes) gl_SNPRINTF_RETVAL_C99 case "$gl_cv_func_snprintf_retval_c99" in *yes) gl_PRINTF_POSITIONS case "$gl_cv_func_printf_positions" in *yes) gl_cv_func_vsnprintf_usable=yes ;; esac ;; esac ;; esac fi if test $gl_cv_func_vsnprintf_usable = no; then gl_REPLACE_VSNPRINTF fi AC_CHECK_DECLS_ONCE([vsnprintf]) if test $ac_cv_have_decl_vsnprintf = no; then HAVE_DECL_VSNPRINTF=0 fi ]) AC_DEFUN([gl_REPLACE_VSNPRINTF], [ AC_REQUIRE([gl_STDIO_H_DEFAULTS]) AC_LIBOBJ([vsnprintf]) if test $ac_cv_func_vsnprintf = yes; then REPLACE_VSNPRINTF=1 fi gl_PREREQ_VSNPRINTF ]) # Prerequisites of lib/vsnprintf.c. AC_DEFUN([gl_PREREQ_VSNPRINTF], [:]) gnuastro-0.2.33-8a3b/bootstrapped/m4/vasnprintf.m40000644000175000017500000002113313004436755016606 00000000000000# vasnprintf.m4 serial 36 dnl Copyright (C) 2002-2004, 2006-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_VASNPRINTF], [ AC_CHECK_FUNCS_ONCE([vasnprintf]) if test $ac_cv_func_vasnprintf = no; then gl_REPLACE_VASNPRINTF fi ]) AC_DEFUN([gl_REPLACE_VASNPRINTF], [ AC_CHECK_FUNCS_ONCE([vasnprintf]) AC_LIBOBJ([vasnprintf]) AC_LIBOBJ([printf-args]) AC_LIBOBJ([printf-parse]) AC_LIBOBJ([asnprintf]) if test $ac_cv_func_vasnprintf = yes; then AC_DEFINE([REPLACE_VASNPRINTF], [1], [Define if vasnprintf exists but is overridden by gnulib.]) fi gl_PREREQ_PRINTF_ARGS gl_PREREQ_PRINTF_PARSE gl_PREREQ_VASNPRINTF gl_PREREQ_ASNPRINTF ]) # Prerequisites of lib/printf-args.h, lib/printf-args.c. AC_DEFUN([gl_PREREQ_PRINTF_ARGS], [ AC_REQUIRE([AC_TYPE_LONG_LONG_INT]) AC_REQUIRE([gt_TYPE_WCHAR_T]) AC_REQUIRE([gt_TYPE_WINT_T]) ]) # Prerequisites of lib/printf-parse.h, lib/printf-parse.c. AC_DEFUN([gl_PREREQ_PRINTF_PARSE], [ AC_REQUIRE([gl_FEATURES_H]) AC_REQUIRE([AC_TYPE_LONG_LONG_INT]) AC_REQUIRE([gt_TYPE_WCHAR_T]) AC_REQUIRE([gt_TYPE_WINT_T]) AC_REQUIRE([AC_TYPE_SIZE_T]) AC_CHECK_TYPE([ptrdiff_t], , [AC_DEFINE([ptrdiff_t], [long], [Define as the type of the result of subtracting two pointers, if the system doesn't define it.]) ]) AC_REQUIRE([gt_AC_TYPE_INTMAX_T]) ]) # Prerequisites of lib/vasnprintf.c. AC_DEFUN_ONCE([gl_PREREQ_VASNPRINTF], [ AC_REQUIRE([AC_FUNC_ALLOCA]) AC_REQUIRE([AC_TYPE_LONG_LONG_INT]) AC_REQUIRE([gt_TYPE_WCHAR_T]) AC_REQUIRE([gt_TYPE_WINT_T]) AC_CHECK_FUNCS([snprintf strnlen wcslen wcsnlen mbrtowc wcrtomb]) dnl Use the _snprintf function only if it is declared (because on NetBSD it dnl is defined as a weak alias of snprintf; we prefer to use the latter). AC_CHECK_DECLS([_snprintf], , , [[#include ]]) dnl Knowing DBL_EXPBIT0_WORD and DBL_EXPBIT0_BIT enables an optimization dnl in the code for NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_DOUBLE. AC_REQUIRE([gl_DOUBLE_EXPONENT_LOCATION]) dnl We can avoid a lot of code by assuming that snprintf's return value dnl conforms to ISO C99. So check that. AC_REQUIRE([gl_SNPRINTF_RETVAL_C99]) case "$gl_cv_func_snprintf_retval_c99" in *yes) AC_DEFINE([HAVE_SNPRINTF_RETVAL_C99], [1], [Define if the return value of the snprintf function is the number of of bytes (excluding the terminating NUL) that would have been produced if the buffer had been large enough.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting 'long double' # arguments. AC_DEFUN_ONCE([gl_PREREQ_VASNPRINTF_LONG_DOUBLE], [ AC_REQUIRE([gl_PRINTF_LONG_DOUBLE]) case "$gl_cv_func_printf_long_double" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_LONG_DOUBLE], [1], [Define if the vasnprintf implementation needs special code for 'long double' arguments.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting infinite 'double' # arguments. AC_DEFUN([gl_PREREQ_VASNPRINTF_INFINITE_DOUBLE], [ AC_REQUIRE([gl_PRINTF_INFINITE]) case "$gl_cv_func_printf_infinite" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_INFINITE_DOUBLE], [1], [Define if the vasnprintf implementation needs special code for infinite 'double' arguments.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting infinite 'long double' # arguments. AC_DEFUN([gl_PREREQ_VASNPRINTF_INFINITE_LONG_DOUBLE], [ AC_REQUIRE([gl_PRINTF_INFINITE_LONG_DOUBLE]) dnl There is no need to set NEED_PRINTF_INFINITE_LONG_DOUBLE if dnl NEED_PRINTF_LONG_DOUBLE is already set. AC_REQUIRE([gl_PREREQ_VASNPRINTF_LONG_DOUBLE]) case "$gl_cv_func_printf_long_double" in *yes) case "$gl_cv_func_printf_infinite_long_double" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_INFINITE_LONG_DOUBLE], [1], [Define if the vasnprintf implementation needs special code for infinite 'long double' arguments.]) ;; esac ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting the 'a' directive. AC_DEFUN([gl_PREREQ_VASNPRINTF_DIRECTIVE_A], [ AC_REQUIRE([gl_PRINTF_DIRECTIVE_A]) case "$gl_cv_func_printf_directive_a" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_DIRECTIVE_A], [1], [Define if the vasnprintf implementation needs special code for the 'a' and 'A' directives.]) AC_CHECK_FUNCS([nl_langinfo]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting the 'F' directive. AC_DEFUN([gl_PREREQ_VASNPRINTF_DIRECTIVE_F], [ AC_REQUIRE([gl_PRINTF_DIRECTIVE_F]) case "$gl_cv_func_printf_directive_f" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_DIRECTIVE_F], [1], [Define if the vasnprintf implementation needs special code for the 'F' directive.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting the 'ls' directive. AC_DEFUN([gl_PREREQ_VASNPRINTF_DIRECTIVE_LS], [ AC_REQUIRE([gl_PRINTF_DIRECTIVE_LS]) case "$gl_cv_func_printf_directive_ls" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_DIRECTIVE_LS], [1], [Define if the vasnprintf implementation needs special code for the 'ls' directive.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting the ' flag. AC_DEFUN([gl_PREREQ_VASNPRINTF_FLAG_GROUPING], [ AC_REQUIRE([gl_PRINTF_FLAG_GROUPING]) case "$gl_cv_func_printf_flag_grouping" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_FLAG_GROUPING], [1], [Define if the vasnprintf implementation needs special code for the ' flag.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting the '-' flag. AC_DEFUN([gl_PREREQ_VASNPRINTF_FLAG_LEFTADJUST], [ AC_REQUIRE([gl_PRINTF_FLAG_LEFTADJUST]) case "$gl_cv_func_printf_flag_leftadjust" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_FLAG_LEFTADJUST], [1], [Define if the vasnprintf implementation needs special code for the '-' flag.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting the 0 flag. AC_DEFUN([gl_PREREQ_VASNPRINTF_FLAG_ZERO], [ AC_REQUIRE([gl_PRINTF_FLAG_ZERO]) case "$gl_cv_func_printf_flag_zero" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_FLAG_ZERO], [1], [Define if the vasnprintf implementation needs special code for the 0 flag.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting large precisions. AC_DEFUN([gl_PREREQ_VASNPRINTF_PRECISION], [ AC_REQUIRE([gl_PRINTF_PRECISION]) case "$gl_cv_func_printf_precision" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_UNBOUNDED_PRECISION], [1], [Define if the vasnprintf implementation needs special code for supporting large precisions without arbitrary bounds.]) AC_DEFINE([NEED_PRINTF_DOUBLE], [1], [Define if the vasnprintf implementation needs special code for 'double' arguments.]) AC_DEFINE([NEED_PRINTF_LONG_DOUBLE], [1], [Define if the vasnprintf implementation needs special code for 'long double' arguments.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for surviving out-of-memory # conditions. AC_DEFUN([gl_PREREQ_VASNPRINTF_ENOMEM], [ AC_REQUIRE([gl_PRINTF_ENOMEM]) case "$gl_cv_func_printf_enomem" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_ENOMEM], [1], [Define if the vasnprintf implementation needs special code for surviving out-of-memory conditions.]) AC_DEFINE([NEED_PRINTF_DOUBLE], [1], [Define if the vasnprintf implementation needs special code for 'double' arguments.]) AC_DEFINE([NEED_PRINTF_LONG_DOUBLE], [1], [Define if the vasnprintf implementation needs special code for 'long double' arguments.]) ;; esac ]) # Prerequisites of lib/vasnprintf.c including all extras for POSIX compliance. AC_DEFUN([gl_PREREQ_VASNPRINTF_WITH_EXTRAS], [ AC_REQUIRE([gl_PREREQ_VASNPRINTF]) gl_PREREQ_VASNPRINTF_LONG_DOUBLE gl_PREREQ_VASNPRINTF_INFINITE_DOUBLE gl_PREREQ_VASNPRINTF_INFINITE_LONG_DOUBLE gl_PREREQ_VASNPRINTF_DIRECTIVE_A gl_PREREQ_VASNPRINTF_DIRECTIVE_F gl_PREREQ_VASNPRINTF_DIRECTIVE_LS gl_PREREQ_VASNPRINTF_FLAG_GROUPING gl_PREREQ_VASNPRINTF_FLAG_LEFTADJUST gl_PREREQ_VASNPRINTF_FLAG_ZERO gl_PREREQ_VASNPRINTF_PRECISION gl_PREREQ_VASNPRINTF_ENOMEM ]) # Prerequisites of lib/asnprintf.c. AC_DEFUN([gl_PREREQ_ASNPRINTF], [ ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/unistd_h.m40000644000175000017500000002171213004436755016234 00000000000000# unistd_h.m4 serial 68 dnl Copyright (C) 2006-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Written by Simon Josefsson, Bruno Haible. AC_DEFUN([gl_UNISTD_H], [ dnl Use AC_REQUIRE here, so that the default behavior below is expanded dnl once only, before all statements that occur in other macros. AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) gl_CHECK_NEXT_HEADERS([unistd.h]) if test $ac_cv_header_unistd_h = yes; then HAVE_UNISTD_H=1 else HAVE_UNISTD_H=0 fi AC_SUBST([HAVE_UNISTD_H]) dnl Ensure the type pid_t gets defined. AC_REQUIRE([AC_TYPE_PID_T]) dnl Determine WINDOWS_64_BIT_OFF_T. AC_REQUIRE([gl_TYPE_OFF_T]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[ #if HAVE_UNISTD_H # include #endif /* Some systems declare various items in the wrong headers. */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include # include # include # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # include # endif #endif ]], [chdir chown dup dup2 dup3 environ euidaccess faccessat fchdir fchownat fdatasync fsync ftruncate getcwd getdomainname getdtablesize getgroups gethostname getlogin getlogin_r getpagesize getusershell setusershell endusershell group_member isatty lchown link linkat lseek pipe pipe2 pread pwrite readlink readlinkat rmdir sethostname sleep symlink symlinkat ttyname_r unlink unlinkat usleep]) ]) AC_DEFUN([gl_UNISTD_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_UNISTD_H_DEFAULTS], [ GNULIB_CHDIR=0; AC_SUBST([GNULIB_CHDIR]) GNULIB_CHOWN=0; AC_SUBST([GNULIB_CHOWN]) GNULIB_CLOSE=0; AC_SUBST([GNULIB_CLOSE]) GNULIB_DUP=0; AC_SUBST([GNULIB_DUP]) GNULIB_DUP2=0; AC_SUBST([GNULIB_DUP2]) GNULIB_DUP3=0; AC_SUBST([GNULIB_DUP3]) GNULIB_ENVIRON=0; AC_SUBST([GNULIB_ENVIRON]) GNULIB_EUIDACCESS=0; AC_SUBST([GNULIB_EUIDACCESS]) GNULIB_FACCESSAT=0; AC_SUBST([GNULIB_FACCESSAT]) GNULIB_FCHDIR=0; AC_SUBST([GNULIB_FCHDIR]) GNULIB_FCHOWNAT=0; AC_SUBST([GNULIB_FCHOWNAT]) GNULIB_FDATASYNC=0; AC_SUBST([GNULIB_FDATASYNC]) GNULIB_FSYNC=0; AC_SUBST([GNULIB_FSYNC]) GNULIB_FTRUNCATE=0; AC_SUBST([GNULIB_FTRUNCATE]) GNULIB_GETCWD=0; AC_SUBST([GNULIB_GETCWD]) GNULIB_GETDOMAINNAME=0; AC_SUBST([GNULIB_GETDOMAINNAME]) GNULIB_GETDTABLESIZE=0; AC_SUBST([GNULIB_GETDTABLESIZE]) GNULIB_GETGROUPS=0; AC_SUBST([GNULIB_GETGROUPS]) GNULIB_GETHOSTNAME=0; AC_SUBST([GNULIB_GETHOSTNAME]) GNULIB_GETLOGIN=0; AC_SUBST([GNULIB_GETLOGIN]) GNULIB_GETLOGIN_R=0; AC_SUBST([GNULIB_GETLOGIN_R]) GNULIB_GETPAGESIZE=0; AC_SUBST([GNULIB_GETPAGESIZE]) GNULIB_GETUSERSHELL=0; AC_SUBST([GNULIB_GETUSERSHELL]) GNULIB_GROUP_MEMBER=0; AC_SUBST([GNULIB_GROUP_MEMBER]) GNULIB_ISATTY=0; AC_SUBST([GNULIB_ISATTY]) GNULIB_LCHOWN=0; AC_SUBST([GNULIB_LCHOWN]) GNULIB_LINK=0; AC_SUBST([GNULIB_LINK]) GNULIB_LINKAT=0; AC_SUBST([GNULIB_LINKAT]) GNULIB_LSEEK=0; AC_SUBST([GNULIB_LSEEK]) GNULIB_PIPE=0; AC_SUBST([GNULIB_PIPE]) GNULIB_PIPE2=0; AC_SUBST([GNULIB_PIPE2]) GNULIB_PREAD=0; AC_SUBST([GNULIB_PREAD]) GNULIB_PWRITE=0; AC_SUBST([GNULIB_PWRITE]) GNULIB_READ=0; AC_SUBST([GNULIB_READ]) GNULIB_READLINK=0; AC_SUBST([GNULIB_READLINK]) GNULIB_READLINKAT=0; AC_SUBST([GNULIB_READLINKAT]) GNULIB_RMDIR=0; AC_SUBST([GNULIB_RMDIR]) GNULIB_SETHOSTNAME=0; AC_SUBST([GNULIB_SETHOSTNAME]) GNULIB_SLEEP=0; AC_SUBST([GNULIB_SLEEP]) GNULIB_SYMLINK=0; AC_SUBST([GNULIB_SYMLINK]) GNULIB_SYMLINKAT=0; AC_SUBST([GNULIB_SYMLINKAT]) GNULIB_TTYNAME_R=0; AC_SUBST([GNULIB_TTYNAME_R]) GNULIB_UNISTD_H_NONBLOCKING=0; AC_SUBST([GNULIB_UNISTD_H_NONBLOCKING]) GNULIB_UNISTD_H_SIGPIPE=0; AC_SUBST([GNULIB_UNISTD_H_SIGPIPE]) GNULIB_UNLINK=0; AC_SUBST([GNULIB_UNLINK]) GNULIB_UNLINKAT=0; AC_SUBST([GNULIB_UNLINKAT]) GNULIB_USLEEP=0; AC_SUBST([GNULIB_USLEEP]) GNULIB_WRITE=0; AC_SUBST([GNULIB_WRITE]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_CHOWN=1; AC_SUBST([HAVE_CHOWN]) HAVE_DUP2=1; AC_SUBST([HAVE_DUP2]) HAVE_DUP3=1; AC_SUBST([HAVE_DUP3]) HAVE_EUIDACCESS=1; AC_SUBST([HAVE_EUIDACCESS]) HAVE_FACCESSAT=1; AC_SUBST([HAVE_FACCESSAT]) HAVE_FCHDIR=1; AC_SUBST([HAVE_FCHDIR]) HAVE_FCHOWNAT=1; AC_SUBST([HAVE_FCHOWNAT]) HAVE_FDATASYNC=1; AC_SUBST([HAVE_FDATASYNC]) HAVE_FSYNC=1; AC_SUBST([HAVE_FSYNC]) HAVE_FTRUNCATE=1; AC_SUBST([HAVE_FTRUNCATE]) HAVE_GETDTABLESIZE=1; AC_SUBST([HAVE_GETDTABLESIZE]) HAVE_GETGROUPS=1; AC_SUBST([HAVE_GETGROUPS]) HAVE_GETHOSTNAME=1; AC_SUBST([HAVE_GETHOSTNAME]) HAVE_GETLOGIN=1; AC_SUBST([HAVE_GETLOGIN]) HAVE_GETPAGESIZE=1; AC_SUBST([HAVE_GETPAGESIZE]) HAVE_GROUP_MEMBER=1; AC_SUBST([HAVE_GROUP_MEMBER]) HAVE_LCHOWN=1; AC_SUBST([HAVE_LCHOWN]) HAVE_LINK=1; AC_SUBST([HAVE_LINK]) HAVE_LINKAT=1; AC_SUBST([HAVE_LINKAT]) HAVE_PIPE=1; AC_SUBST([HAVE_PIPE]) HAVE_PIPE2=1; AC_SUBST([HAVE_PIPE2]) HAVE_PREAD=1; AC_SUBST([HAVE_PREAD]) HAVE_PWRITE=1; AC_SUBST([HAVE_PWRITE]) HAVE_READLINK=1; AC_SUBST([HAVE_READLINK]) HAVE_READLINKAT=1; AC_SUBST([HAVE_READLINKAT]) HAVE_SETHOSTNAME=1; AC_SUBST([HAVE_SETHOSTNAME]) HAVE_SLEEP=1; AC_SUBST([HAVE_SLEEP]) HAVE_SYMLINK=1; AC_SUBST([HAVE_SYMLINK]) HAVE_SYMLINKAT=1; AC_SUBST([HAVE_SYMLINKAT]) HAVE_UNLINKAT=1; AC_SUBST([HAVE_UNLINKAT]) HAVE_USLEEP=1; AC_SUBST([HAVE_USLEEP]) HAVE_DECL_ENVIRON=1; AC_SUBST([HAVE_DECL_ENVIRON]) HAVE_DECL_FCHDIR=1; AC_SUBST([HAVE_DECL_FCHDIR]) HAVE_DECL_FDATASYNC=1; AC_SUBST([HAVE_DECL_FDATASYNC]) HAVE_DECL_GETDOMAINNAME=1; AC_SUBST([HAVE_DECL_GETDOMAINNAME]) HAVE_DECL_GETLOGIN_R=1; AC_SUBST([HAVE_DECL_GETLOGIN_R]) HAVE_DECL_GETPAGESIZE=1; AC_SUBST([HAVE_DECL_GETPAGESIZE]) HAVE_DECL_GETUSERSHELL=1; AC_SUBST([HAVE_DECL_GETUSERSHELL]) HAVE_DECL_SETHOSTNAME=1; AC_SUBST([HAVE_DECL_SETHOSTNAME]) HAVE_DECL_TTYNAME_R=1; AC_SUBST([HAVE_DECL_TTYNAME_R]) HAVE_OS_H=0; AC_SUBST([HAVE_OS_H]) HAVE_SYS_PARAM_H=0; AC_SUBST([HAVE_SYS_PARAM_H]) REPLACE_CHOWN=0; AC_SUBST([REPLACE_CHOWN]) REPLACE_CLOSE=0; AC_SUBST([REPLACE_CLOSE]) REPLACE_DUP=0; AC_SUBST([REPLACE_DUP]) REPLACE_DUP2=0; AC_SUBST([REPLACE_DUP2]) REPLACE_FCHOWNAT=0; AC_SUBST([REPLACE_FCHOWNAT]) REPLACE_FTRUNCATE=0; AC_SUBST([REPLACE_FTRUNCATE]) REPLACE_GETCWD=0; AC_SUBST([REPLACE_GETCWD]) REPLACE_GETDOMAINNAME=0; AC_SUBST([REPLACE_GETDOMAINNAME]) REPLACE_GETDTABLESIZE=0; AC_SUBST([REPLACE_GETDTABLESIZE]) REPLACE_GETLOGIN_R=0; AC_SUBST([REPLACE_GETLOGIN_R]) REPLACE_GETGROUPS=0; AC_SUBST([REPLACE_GETGROUPS]) REPLACE_GETPAGESIZE=0; AC_SUBST([REPLACE_GETPAGESIZE]) REPLACE_ISATTY=0; AC_SUBST([REPLACE_ISATTY]) REPLACE_LCHOWN=0; AC_SUBST([REPLACE_LCHOWN]) REPLACE_LINK=0; AC_SUBST([REPLACE_LINK]) REPLACE_LINKAT=0; AC_SUBST([REPLACE_LINKAT]) REPLACE_LSEEK=0; AC_SUBST([REPLACE_LSEEK]) REPLACE_PREAD=0; AC_SUBST([REPLACE_PREAD]) REPLACE_PWRITE=0; AC_SUBST([REPLACE_PWRITE]) REPLACE_READ=0; AC_SUBST([REPLACE_READ]) REPLACE_READLINK=0; AC_SUBST([REPLACE_READLINK]) REPLACE_READLINKAT=0; AC_SUBST([REPLACE_READLINKAT]) REPLACE_RMDIR=0; AC_SUBST([REPLACE_RMDIR]) REPLACE_SLEEP=0; AC_SUBST([REPLACE_SLEEP]) REPLACE_SYMLINK=0; AC_SUBST([REPLACE_SYMLINK]) REPLACE_SYMLINKAT=0; AC_SUBST([REPLACE_SYMLINKAT]) REPLACE_TTYNAME_R=0; AC_SUBST([REPLACE_TTYNAME_R]) REPLACE_UNLINK=0; AC_SUBST([REPLACE_UNLINK]) REPLACE_UNLINKAT=0; AC_SUBST([REPLACE_UNLINKAT]) REPLACE_USLEEP=0; AC_SUBST([REPLACE_USLEEP]) REPLACE_WRITE=0; AC_SUBST([REPLACE_WRITE]) UNISTD_H_HAVE_WINSOCK2_H=0; AC_SUBST([UNISTD_H_HAVE_WINSOCK2_H]) UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS=0; AC_SUBST([UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/time_h.m40000644000175000017500000001253713004436755015671 00000000000000# Configure a more-standard replacement for . # Copyright (C) 2000-2001, 2003-2007, 2009-2016 Free Software Foundation, Inc. # serial 9 # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # Written by Paul Eggert and Jim Meyering. AC_DEFUN([gl_HEADER_TIME_H], [ dnl Use AC_REQUIRE here, so that the default behavior below is expanded dnl once only, before all statements that occur in other macros. AC_REQUIRE([gl_HEADER_TIME_H_BODY]) ]) AC_DEFUN([gl_HEADER_TIME_H_BODY], [ AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([gl_HEADER_TIME_H_DEFAULTS]) gl_NEXT_HEADERS([time.h]) AC_REQUIRE([gl_CHECK_TYPE_STRUCT_TIMESPEC]) ]) dnl Check whether 'struct timespec' is declared dnl in time.h, sys/time.h, pthread.h, or unistd.h. AC_DEFUN([gl_CHECK_TYPE_STRUCT_TIMESPEC], [ AC_CHECK_HEADERS_ONCE([sys/time.h]) AC_CACHE_CHECK([for struct timespec in ], [gl_cv_sys_struct_timespec_in_time_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[static struct timespec x; x.tv_sec = x.tv_nsec;]])], [gl_cv_sys_struct_timespec_in_time_h=yes], [gl_cv_sys_struct_timespec_in_time_h=no])]) TIME_H_DEFINES_STRUCT_TIMESPEC=0 SYS_TIME_H_DEFINES_STRUCT_TIMESPEC=0 PTHREAD_H_DEFINES_STRUCT_TIMESPEC=0 UNISTD_H_DEFINES_STRUCT_TIMESPEC=0 if test $gl_cv_sys_struct_timespec_in_time_h = yes; then TIME_H_DEFINES_STRUCT_TIMESPEC=1 else AC_CACHE_CHECK([for struct timespec in ], [gl_cv_sys_struct_timespec_in_sys_time_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[static struct timespec x; x.tv_sec = x.tv_nsec;]])], [gl_cv_sys_struct_timespec_in_sys_time_h=yes], [gl_cv_sys_struct_timespec_in_sys_time_h=no])]) if test $gl_cv_sys_struct_timespec_in_sys_time_h = yes; then SYS_TIME_H_DEFINES_STRUCT_TIMESPEC=1 else AC_CACHE_CHECK([for struct timespec in ], [gl_cv_sys_struct_timespec_in_pthread_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[static struct timespec x; x.tv_sec = x.tv_nsec;]])], [gl_cv_sys_struct_timespec_in_pthread_h=yes], [gl_cv_sys_struct_timespec_in_pthread_h=no])]) if test $gl_cv_sys_struct_timespec_in_pthread_h = yes; then PTHREAD_H_DEFINES_STRUCT_TIMESPEC=1 else AC_CACHE_CHECK([for struct timespec in ], [gl_cv_sys_struct_timespec_in_unistd_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[static struct timespec x; x.tv_sec = x.tv_nsec;]])], [gl_cv_sys_struct_timespec_in_unistd_h=yes], [gl_cv_sys_struct_timespec_in_unistd_h=no])]) if test $gl_cv_sys_struct_timespec_in_unistd_h = yes; then UNISTD_H_DEFINES_STRUCT_TIMESPEC=1 fi fi fi fi AC_SUBST([TIME_H_DEFINES_STRUCT_TIMESPEC]) AC_SUBST([SYS_TIME_H_DEFINES_STRUCT_TIMESPEC]) AC_SUBST([PTHREAD_H_DEFINES_STRUCT_TIMESPEC]) AC_SUBST([UNISTD_H_DEFINES_STRUCT_TIMESPEC]) ]) AC_DEFUN([gl_TIME_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_HEADER_TIME_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_HEADER_TIME_H_DEFAULTS], [ GNULIB_MKTIME=0; AC_SUBST([GNULIB_MKTIME]) GNULIB_NANOSLEEP=0; AC_SUBST([GNULIB_NANOSLEEP]) GNULIB_STRPTIME=0; AC_SUBST([GNULIB_STRPTIME]) GNULIB_TIMEGM=0; AC_SUBST([GNULIB_TIMEGM]) GNULIB_TIME_R=0; AC_SUBST([GNULIB_TIME_R]) GNULIB_TIME_RZ=0; AC_SUBST([GNULIB_TIME_RZ]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_DECL_LOCALTIME_R=1; AC_SUBST([HAVE_DECL_LOCALTIME_R]) HAVE_NANOSLEEP=1; AC_SUBST([HAVE_NANOSLEEP]) HAVE_STRPTIME=1; AC_SUBST([HAVE_STRPTIME]) HAVE_TIMEGM=1; AC_SUBST([HAVE_TIMEGM]) dnl If another module says to replace or to not replace, do that. dnl Otherwise, replace only if someone compiles with -DGNULIB_PORTCHECK; dnl this lets maintainers check for portability. REPLACE_LOCALTIME_R=GNULIB_PORTCHECK; AC_SUBST([REPLACE_LOCALTIME_R]) REPLACE_MKTIME=GNULIB_PORTCHECK; AC_SUBST([REPLACE_MKTIME]) REPLACE_NANOSLEEP=GNULIB_PORTCHECK; AC_SUBST([REPLACE_NANOSLEEP]) REPLACE_TIMEGM=GNULIB_PORTCHECK; AC_SUBST([REPLACE_TIMEGM]) dnl Hack so that the time module doesn't depend on the sys_time module. dnl First, default GNULIB_GETTIMEOFDAY to 0 if sys_time is absent. : ${GNULIB_GETTIMEOFDAY=0}; AC_SUBST([GNULIB_GETTIMEOFDAY]) dnl Second, it's OK to not use GNULIB_PORTCHECK for REPLACE_GMTIME dnl and REPLACE_LOCALTIME, as portability to Solaris 2.6 and earlier dnl is no longer a big deal. REPLACE_GMTIME=0; AC_SUBST([REPLACE_GMTIME]) REPLACE_LOCALTIME=0; AC_SUBST([REPLACE_LOCALTIME]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/threadlib.m40000644000175000017500000003545713004436755016370 00000000000000# threadlib.m4 serial 11 (gettext-0.18.2) dnl Copyright (C) 2005-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl gl_THREADLIB dnl ------------ dnl Tests for a multithreading library to be used. dnl If the configure.ac contains a definition of the gl_THREADLIB_DEFAULT_NO dnl (it must be placed before the invocation of gl_THREADLIB_EARLY!), then the dnl default is 'no', otherwise it is system dependent. In both cases, the user dnl can change the choice through the options --enable-threads=choice or dnl --disable-threads. dnl Defines at most one of the macros USE_POSIX_THREADS, USE_SOLARIS_THREADS, dnl USE_PTH_THREADS, USE_WINDOWS_THREADS dnl Sets the variables LIBTHREAD and LTLIBTHREAD to the linker options for use dnl in a Makefile (LIBTHREAD for use without libtool, LTLIBTHREAD for use with dnl libtool). dnl Sets the variables LIBMULTITHREAD and LTLIBMULTITHREAD similarly, for dnl programs that really need multithread functionality. The difference dnl between LIBTHREAD and LIBMULTITHREAD is that on platforms supporting weak dnl symbols, typically LIBTHREAD is empty whereas LIBMULTITHREAD is not. dnl Adds to CPPFLAGS the flag -D_REENTRANT or -D_THREAD_SAFE if needed for dnl multithread-safe programs. AC_DEFUN([gl_THREADLIB_EARLY], [ AC_REQUIRE([gl_THREADLIB_EARLY_BODY]) ]) dnl The guts of gl_THREADLIB_EARLY. Needs to be expanded only once. AC_DEFUN([gl_THREADLIB_EARLY_BODY], [ dnl Ordering constraints: This macro modifies CPPFLAGS in a way that dnl influences the result of the autoconf tests that test for *_unlocked dnl declarations, on AIX 5 at least. Therefore it must come early. AC_BEFORE([$0], [gl_FUNC_GLIBC_UNLOCKED_IO])dnl AC_BEFORE([$0], [gl_ARGP])dnl AC_REQUIRE([AC_CANONICAL_HOST]) dnl _GNU_SOURCE is needed for pthread_rwlock_t on glibc systems. dnl AC_USE_SYSTEM_EXTENSIONS was introduced in autoconf 2.60 and obsoletes dnl AC_GNU_SOURCE. m4_ifdef([AC_USE_SYSTEM_EXTENSIONS], [AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS])], [AC_REQUIRE([AC_GNU_SOURCE])]) dnl Check for multithreading. m4_ifdef([gl_THREADLIB_DEFAULT_NO], [m4_divert_text([DEFAULTS], [gl_use_threads_default=no])], [m4_divert_text([DEFAULTS], [gl_use_threads_default=])]) AC_ARG_ENABLE([threads], AC_HELP_STRING([--enable-threads={posix|solaris|pth|windows}], [specify multithreading API])m4_ifdef([gl_THREADLIB_DEFAULT_NO], [], [ AC_HELP_STRING([--disable-threads], [build without multithread safety])]), [gl_use_threads=$enableval], [if test -n "$gl_use_threads_default"; then gl_use_threads="$gl_use_threads_default" else changequote(,)dnl case "$host_os" in dnl Disable multithreading by default on OSF/1, because it interferes dnl with fork()/exec(): When msgexec is linked with -lpthread, its dnl child process gets an endless segmentation fault inside execvp(). dnl Disable multithreading by default on Cygwin 1.5.x, because it has dnl bugs that lead to endless loops or crashes. See dnl . osf*) gl_use_threads=no ;; cygwin*) case `uname -r` in 1.[0-5].*) gl_use_threads=no ;; *) gl_use_threads=yes ;; esac ;; *) gl_use_threads=yes ;; esac changequote([,])dnl fi ]) if test "$gl_use_threads" = yes || test "$gl_use_threads" = posix; then # For using : case "$host_os" in osf*) # On OSF/1, the compiler needs the flag -D_REENTRANT so that it # groks . cc also understands the flag -pthread, but # we don't use it because 1. gcc-2.95 doesn't understand -pthread, # 2. putting a flag into CPPFLAGS that has an effect on the linker # causes the AC_LINK_IFELSE test below to succeed unexpectedly, # leading to wrong values of LIBTHREAD and LTLIBTHREAD. CPPFLAGS="$CPPFLAGS -D_REENTRANT" ;; esac # Some systems optimize for single-threaded programs by default, and # need special flags to disable these optimizations. For example, the # definition of 'errno' in . case "$host_os" in aix* | freebsd*) CPPFLAGS="$CPPFLAGS -D_THREAD_SAFE" ;; solaris*) CPPFLAGS="$CPPFLAGS -D_REENTRANT" ;; esac fi ]) dnl The guts of gl_THREADLIB. Needs to be expanded only once. AC_DEFUN([gl_THREADLIB_BODY], [ AC_REQUIRE([gl_THREADLIB_EARLY_BODY]) gl_threads_api=none LIBTHREAD= LTLIBTHREAD= LIBMULTITHREAD= LTLIBMULTITHREAD= if test "$gl_use_threads" != no; then dnl Check whether the compiler and linker support weak declarations. AC_CACHE_CHECK([whether imported symbols can be declared weak], [gl_cv_have_weak], [gl_cv_have_weak=no dnl First, test whether the compiler accepts it syntactically. AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[extern void xyzzy (); #pragma weak xyzzy]], [[xyzzy();]])], [gl_cv_have_weak=maybe]) if test $gl_cv_have_weak = maybe; then dnl Second, test whether it actually works. On Cygwin 1.7.2, with dnl gcc 4.3, symbols declared weak always evaluate to the address 0. AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #pragma weak fputs int main () { return (fputs == NULL); }]])], [gl_cv_have_weak=yes], [gl_cv_have_weak=no], [dnl When cross-compiling, assume that only ELF platforms support dnl weak symbols. AC_EGREP_CPP([Extensible Linking Format], [#ifdef __ELF__ Extensible Linking Format #endif ], [gl_cv_have_weak="guessing yes"], [gl_cv_have_weak="guessing no"]) ]) fi ]) if test "$gl_use_threads" = yes || test "$gl_use_threads" = posix; then # On OSF/1, the compiler needs the flag -pthread or -D_REENTRANT so that # it groks . It's added above, in gl_THREADLIB_EARLY_BODY. AC_CHECK_HEADER([pthread.h], [gl_have_pthread_h=yes], [gl_have_pthread_h=no]) if test "$gl_have_pthread_h" = yes; then # Other possible tests: # -lpthreads (FSU threads, PCthreads) # -lgthreads gl_have_pthread= # Test whether both pthread_mutex_lock and pthread_mutexattr_init exist # in libc. IRIX 6.5 has the first one in both libc and libpthread, but # the second one only in libpthread, and lock.c needs it. # # If -pthread works, prefer it to -lpthread, since Ubuntu 14.04 # needs -pthread for some reason. See: # http://lists.gnu.org/archive/html/bug-gnulib/2014-09/msg00023.html save_LIBS=$LIBS for gl_pthread in '' '-pthread'; do LIBS="$LIBS $gl_pthread" AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include pthread_mutex_t m; pthread_mutexattr_t ma; ]], [[pthread_mutex_lock (&m); pthread_mutexattr_init (&ma);]])], [gl_have_pthread=yes LIBTHREAD=$gl_pthread LTLIBTHREAD=$gl_pthread LIBMULTITHREAD=$gl_pthread LTLIBMULTITHREAD=$gl_pthread]) LIBS=$save_LIBS test -n "$gl_have_pthread" && break done # Test for libpthread by looking for pthread_kill. (Not pthread_self, # since it is defined as a macro on OSF/1.) if test -n "$gl_have_pthread" && test -z "$LIBTHREAD"; then # The program links fine without libpthread. But it may actually # need to link with libpthread in order to create multiple threads. AC_CHECK_LIB([pthread], [pthread_kill], [LIBMULTITHREAD=-lpthread LTLIBMULTITHREAD=-lpthread # On Solaris and HP-UX, most pthread functions exist also in libc. # Therefore pthread_in_use() needs to actually try to create a # thread: pthread_create from libc will fail, whereas # pthread_create will actually create a thread. case "$host_os" in solaris* | hpux*) AC_DEFINE([PTHREAD_IN_USE_DETECTION_HARD], [1], [Define if the pthread_in_use() detection is hard.]) esac ]) elif test -z "$gl_have_pthread"; then # Some library is needed. Try libpthread and libc_r. AC_CHECK_LIB([pthread], [pthread_kill], [gl_have_pthread=yes LIBTHREAD=-lpthread LTLIBTHREAD=-lpthread LIBMULTITHREAD=-lpthread LTLIBMULTITHREAD=-lpthread]) if test -z "$gl_have_pthread"; then # For FreeBSD 4. AC_CHECK_LIB([c_r], [pthread_kill], [gl_have_pthread=yes LIBTHREAD=-lc_r LTLIBTHREAD=-lc_r LIBMULTITHREAD=-lc_r LTLIBMULTITHREAD=-lc_r]) fi fi if test -n "$gl_have_pthread"; then gl_threads_api=posix AC_DEFINE([USE_POSIX_THREADS], [1], [Define if the POSIX multithreading library can be used.]) if test -n "$LIBMULTITHREAD" || test -n "$LTLIBMULTITHREAD"; then if case "$gl_cv_have_weak" in *yes) true;; *) false;; esac; then AC_DEFINE([USE_POSIX_THREADS_WEAK], [1], [Define if references to the POSIX multithreading library should be made weak.]) LIBTHREAD= LTLIBTHREAD= fi fi fi fi fi if test -z "$gl_have_pthread"; then if test "$gl_use_threads" = yes || test "$gl_use_threads" = solaris; then gl_have_solaristhread= gl_save_LIBS="$LIBS" LIBS="$LIBS -lthread" AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[ #include #include ]], [[thr_self();]])], [gl_have_solaristhread=yes]) LIBS="$gl_save_LIBS" if test -n "$gl_have_solaristhread"; then gl_threads_api=solaris LIBTHREAD=-lthread LTLIBTHREAD=-lthread LIBMULTITHREAD="$LIBTHREAD" LTLIBMULTITHREAD="$LTLIBTHREAD" AC_DEFINE([USE_SOLARIS_THREADS], [1], [Define if the old Solaris multithreading library can be used.]) if case "$gl_cv_have_weak" in *yes) true;; *) false;; esac; then AC_DEFINE([USE_SOLARIS_THREADS_WEAK], [1], [Define if references to the old Solaris multithreading library should be made weak.]) LIBTHREAD= LTLIBTHREAD= fi fi fi fi if test "$gl_use_threads" = pth; then gl_save_CPPFLAGS="$CPPFLAGS" AC_LIB_LINKFLAGS([pth]) gl_have_pth= gl_save_LIBS="$LIBS" LIBS="$LIBS $LIBPTH" AC_LINK_IFELSE( [AC_LANG_PROGRAM([[#include ]], [[pth_self();]])], [gl_have_pth=yes]) LIBS="$gl_save_LIBS" if test -n "$gl_have_pth"; then gl_threads_api=pth LIBTHREAD="$LIBPTH" LTLIBTHREAD="$LTLIBPTH" LIBMULTITHREAD="$LIBTHREAD" LTLIBMULTITHREAD="$LTLIBTHREAD" AC_DEFINE([USE_PTH_THREADS], [1], [Define if the GNU Pth multithreading library can be used.]) if test -n "$LIBMULTITHREAD" || test -n "$LTLIBMULTITHREAD"; then if case "$gl_cv_have_weak" in *yes) true;; *) false;; esac; then AC_DEFINE([USE_PTH_THREADS_WEAK], [1], [Define if references to the GNU Pth multithreading library should be made weak.]) LIBTHREAD= LTLIBTHREAD= fi fi else CPPFLAGS="$gl_save_CPPFLAGS" fi fi if test -z "$gl_have_pthread"; then case "$gl_use_threads" in yes | windows | win32) # The 'win32' is for backward compatibility. if { case "$host_os" in mingw*) true;; *) false;; esac }; then gl_threads_api=windows AC_DEFINE([USE_WINDOWS_THREADS], [1], [Define if the native Windows multithreading API can be used.]) fi ;; esac fi fi AC_MSG_CHECKING([for multithread API to use]) AC_MSG_RESULT([$gl_threads_api]) AC_SUBST([LIBTHREAD]) AC_SUBST([LTLIBTHREAD]) AC_SUBST([LIBMULTITHREAD]) AC_SUBST([LTLIBMULTITHREAD]) ]) AC_DEFUN([gl_THREADLIB], [ AC_REQUIRE([gl_THREADLIB_EARLY]) AC_REQUIRE([gl_THREADLIB_BODY]) ]) dnl gl_DISABLE_THREADS dnl ------------------ dnl Sets the gl_THREADLIB default so that threads are not used by default. dnl The user can still override it at installation time, by using the dnl configure option '--enable-threads'. AC_DEFUN([gl_DISABLE_THREADS], [ m4_divert_text([INIT_PREPARE], [gl_use_threads_default=no]) ]) dnl Survey of platforms: dnl dnl Platform Available Compiler Supports test-lock dnl flavours option weak result dnl --------------- --------- --------- -------- --------- dnl Linux 2.4/glibc posix -lpthread Y OK dnl dnl GNU Hurd/glibc posix dnl dnl Ubuntu 14.04 posix -pthread Y OK dnl dnl FreeBSD 5.3 posix -lc_r Y dnl posix -lkse ? Y dnl posix -lpthread ? Y dnl posix -lthr Y dnl dnl FreeBSD 5.2 posix -lc_r Y dnl posix -lkse Y dnl posix -lthr Y dnl dnl FreeBSD 4.0,4.10 posix -lc_r Y OK dnl dnl NetBSD 1.6 -- dnl dnl OpenBSD 3.4 posix -lpthread Y OK dnl dnl Mac OS X 10.[123] posix -lpthread Y OK dnl dnl Solaris 7,8,9 posix -lpthread Y Sol 7,8: 0.0; Sol 9: OK dnl solaris -lthread Y Sol 7,8: 0.0; Sol 9: OK dnl dnl HP-UX 11 posix -lpthread N (cc) OK dnl Y (gcc) dnl dnl IRIX 6.5 posix -lpthread Y 0.5 dnl dnl AIX 4.3,5.1 posix -lpthread N AIX 4: 0.5; AIX 5: OK dnl dnl OSF/1 4.0,5.1 posix -pthread (cc) N OK dnl -lpthread (gcc) Y dnl dnl Cygwin posix -lpthread Y OK dnl dnl Any of the above pth -lpth 0.0 dnl dnl Mingw windows N OK dnl dnl BeOS 5 -- dnl dnl The test-lock result shows what happens if in test-lock.c EXPLICIT_YIELD is dnl turned off: dnl OK if all three tests terminate OK, dnl 0.5 if the first test terminates OK but the second one loops endlessly, dnl 0.0 if the first test already loops endlessly. gnuastro-0.2.33-8a3b/bootstrapped/m4/thread.m40000644000175000017500000000076113004436755015667 00000000000000# thread.m4 serial 3 dnl Copyright (C) 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_THREAD], [ AC_REQUIRE([gl_THREADLIB]) if test $gl_threads_api = posix; then gl_save_LIBS="$LIBS" LIBS="$LIBS $LIBMULTITHREAD" AC_CHECK_FUNCS([pthread_atfork]) LIBS="$gl_save_LIBS" fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/sysexits.m40000644000175000017500000000237313004436755016314 00000000000000# sysexits.m4 serial 6 dnl Copyright (C) 2003, 2005, 2007, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_SYSEXITS], [ AC_CHECK_HEADERS_ONCE([sysexits.h]) if test $ac_cv_header_sysexits_h = yes; then HAVE_SYSEXITS_H=1 gl_CHECK_NEXT_HEADERS([sysexits.h]) AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[#include ]], [[switch (0) { case EX_OK: case EX_USAGE: case EX_DATAERR: case EX_NOINPUT: case EX_NOUSER: case EX_NOHOST: case EX_UNAVAILABLE: case EX_SOFTWARE: case EX_OSERR: case EX_OSFILE: case EX_CANTCREAT: case EX_IOERR: case EX_TEMPFAIL: case EX_PROTOCOL: case EX_NOPERM: case EX_CONFIG: break; } ]])], [SYSEXITS_H=], [SYSEXITS_H=sysexits.h]) else HAVE_SYSEXITS_H=0 SYSEXITS_H=sysexits.h fi AC_SUBST([HAVE_SYSEXITS_H]) AC_SUBST([SYSEXITS_H]) AM_CONDITIONAL([GL_GENERATE_SYSEXITS_H], [test -n "$SYSEXITS_H"]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/sys_types_h.m40000644000175000017500000000261213004436755016766 00000000000000# sys_types_h.m4 serial 6 dnl Copyright (C) 2011-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN_ONCE([gl_SYS_TYPES_H], [ AC_REQUIRE([gl_SYS_TYPES_H_DEFAULTS]) gl_NEXT_HEADERS([sys/types.h]) dnl Ensure the type pid_t gets defined. AC_REQUIRE([AC_TYPE_PID_T]) dnl Ensure the type mode_t gets defined. AC_REQUIRE([AC_TYPE_MODE_T]) dnl Whether to override the 'off_t' type. AC_REQUIRE([gl_TYPE_OFF_T]) ]) AC_DEFUN([gl_SYS_TYPES_H_DEFAULTS], [ ]) # This works around a buggy version in autoconf <= 2.69. # See m4_version_prereq([2.70], [], [ # This is taken from the following Autoconf patch: # http://git.sv.gnu.org/cgit/autoconf.git/commit/?id=e17a30e98 m4_undefine([AC_HEADER_MAJOR]) AC_DEFUN([AC_HEADER_MAJOR], [AC_CHECK_HEADERS_ONCE([sys/types.h]) AC_CHECK_HEADER([sys/mkdev.h], [AC_DEFINE([MAJOR_IN_MKDEV], [1], [Define to 1 if `major', `minor', and `makedev' are declared in .])]) if test $ac_cv_header_sys_mkdev_h = no; then AC_CHECK_HEADER([sys/sysmacros.h], [AC_DEFINE([MAJOR_IN_SYSMACROS], [1], [Define to 1 if `major', `minor', and `makedev' are declared in .])]) fi ]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/sys_time_h.m40000644000175000017500000000743213004436755016565 00000000000000# Configure a replacement for . # serial 8 # Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # Written by Paul Eggert and Martin Lambers. AC_DEFUN([gl_HEADER_SYS_TIME_H], [ dnl Use AC_REQUIRE here, so that the REPLACE_GETTIMEOFDAY=0 statement dnl below is expanded once only, before all REPLACE_GETTIMEOFDAY=1 dnl statements that occur in other macros. AC_REQUIRE([gl_HEADER_SYS_TIME_H_BODY]) ]) AC_DEFUN([gl_HEADER_SYS_TIME_H_BODY], [ AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([gl_HEADER_SYS_TIME_H_DEFAULTS]) AC_CHECK_HEADERS_ONCE([sys/time.h]) gl_CHECK_NEXT_HEADERS([sys/time.h]) if test $ac_cv_header_sys_time_h != yes; then HAVE_SYS_TIME_H=0 fi dnl On native Windows with MSVC, 'struct timeval' is defined in dnl only. So include that header in the list. gl_PREREQ_SYS_H_WINSOCK2 AC_CACHE_CHECK([for struct timeval], [gl_cv_sys_struct_timeval], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#if HAVE_SYS_TIME_H #include #endif #include #if HAVE_WINSOCK2_H # include #endif ]], [[static struct timeval x; x.tv_sec = x.tv_usec;]])], [gl_cv_sys_struct_timeval=yes], [gl_cv_sys_struct_timeval=no]) ]) if test $gl_cv_sys_struct_timeval != yes; then HAVE_STRUCT_TIMEVAL=0 else dnl On native Windows with a 64-bit 'time_t', 'struct timeval' is defined dnl (in and for mingw64, in only dnl for MSVC) with a tv_sec field of type 'long' (32-bit!), which is dnl smaller than the 'time_t' type mandated by POSIX. dnl On OpenBSD 5.1 amd64, tv_sec is 64 bits and time_t 32 bits, but dnl that is good enough. AC_CACHE_CHECK([for wide-enough struct timeval.tv_sec member], [gl_cv_sys_struct_timeval_tv_sec], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#if HAVE_SYS_TIME_H #include #endif #include #if HAVE_WINSOCK2_H # include #endif ]], [[static struct timeval x; typedef int verify_tv_sec_type[ sizeof (time_t) <= sizeof x.tv_sec ? 1 : -1 ]; ]])], [gl_cv_sys_struct_timeval_tv_sec=yes], [gl_cv_sys_struct_timeval_tv_sec=no]) ]) if test $gl_cv_sys_struct_timeval_tv_sec != yes; then REPLACE_STRUCT_TIMEVAL=1 fi fi dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[ #if HAVE_SYS_TIME_H # include #endif #include ]], [gettimeofday]) ]) AC_DEFUN([gl_SYS_TIME_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_HEADER_SYS_TIME_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_HEADER_SYS_TIME_H_DEFAULTS], [ GNULIB_GETTIMEOFDAY=0; AC_SUBST([GNULIB_GETTIMEOFDAY]) dnl Assume POSIX behavior unless another module says otherwise. HAVE_GETTIMEOFDAY=1; AC_SUBST([HAVE_GETTIMEOFDAY]) HAVE_STRUCT_TIMEVAL=1; AC_SUBST([HAVE_STRUCT_TIMEVAL]) HAVE_SYS_TIME_H=1; AC_SUBST([HAVE_SYS_TIME_H]) HAVE_TIMEZONE_T=0; AC_SUBST([HAVE_TIMEZONE_T]) REPLACE_GETTIMEOFDAY=0; AC_SUBST([REPLACE_GETTIMEOFDAY]) REPLACE_STRUCT_TIMEVAL=0; AC_SUBST([REPLACE_STRUCT_TIMEVAL]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/sys_stat_h.m40000644000175000017500000000723613004436755016604 00000000000000# sys_stat_h.m4 serial 28 -*- Autoconf -*- dnl Copyright (C) 2006-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Eric Blake. dnl Provide a GNU-like . AC_DEFUN([gl_HEADER_SYS_STAT_H], [ AC_REQUIRE([gl_SYS_STAT_H_DEFAULTS]) dnl Check for broken stat macros. AC_REQUIRE([AC_HEADER_STAT]) gl_CHECK_NEXT_HEADERS([sys/stat.h]) dnl Ensure the type mode_t gets defined. AC_REQUIRE([AC_TYPE_MODE_T]) dnl Whether to override 'struct stat'. m4_ifdef([gl_LARGEFILE], [ AC_REQUIRE([gl_LARGEFILE]) ], [ WINDOWS_64_BIT_ST_SIZE=0 ]) AC_SUBST([WINDOWS_64_BIT_ST_SIZE]) if test $WINDOWS_64_BIT_ST_SIZE = 1; then AC_DEFINE([_GL_WINDOWS_64_BIT_ST_SIZE], [1], [Define to 1 if Gnulib overrides 'struct stat' on Windows so that struct stat.st_size becomes 64-bit.]) fi dnl Define types that are supposed to be defined in or dnl . AC_CHECK_TYPE([nlink_t], [], [AC_DEFINE([nlink_t], [int], [Define to the type of st_nlink in struct stat, or a supertype.])], [#include #include ]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[#include ]], [fchmodat fstat fstatat futimens lchmod lstat mkdirat mkfifo mkfifoat mknod mknodat stat utimensat]) ]) # gl_HEADER_SYS_STAT_H AC_DEFUN([gl_SYS_STAT_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_SYS_STAT_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_SYS_STAT_H_DEFAULTS], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) dnl for REPLACE_FCHDIR GNULIB_FCHMODAT=0; AC_SUBST([GNULIB_FCHMODAT]) GNULIB_FSTAT=0; AC_SUBST([GNULIB_FSTAT]) GNULIB_FSTATAT=0; AC_SUBST([GNULIB_FSTATAT]) GNULIB_FUTIMENS=0; AC_SUBST([GNULIB_FUTIMENS]) GNULIB_LCHMOD=0; AC_SUBST([GNULIB_LCHMOD]) GNULIB_LSTAT=0; AC_SUBST([GNULIB_LSTAT]) GNULIB_MKDIRAT=0; AC_SUBST([GNULIB_MKDIRAT]) GNULIB_MKFIFO=0; AC_SUBST([GNULIB_MKFIFO]) GNULIB_MKFIFOAT=0; AC_SUBST([GNULIB_MKFIFOAT]) GNULIB_MKNOD=0; AC_SUBST([GNULIB_MKNOD]) GNULIB_MKNODAT=0; AC_SUBST([GNULIB_MKNODAT]) GNULIB_STAT=0; AC_SUBST([GNULIB_STAT]) GNULIB_UTIMENSAT=0; AC_SUBST([GNULIB_UTIMENSAT]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_FCHMODAT=1; AC_SUBST([HAVE_FCHMODAT]) HAVE_FSTATAT=1; AC_SUBST([HAVE_FSTATAT]) HAVE_FUTIMENS=1; AC_SUBST([HAVE_FUTIMENS]) HAVE_LCHMOD=1; AC_SUBST([HAVE_LCHMOD]) HAVE_LSTAT=1; AC_SUBST([HAVE_LSTAT]) HAVE_MKDIRAT=1; AC_SUBST([HAVE_MKDIRAT]) HAVE_MKFIFO=1; AC_SUBST([HAVE_MKFIFO]) HAVE_MKFIFOAT=1; AC_SUBST([HAVE_MKFIFOAT]) HAVE_MKNOD=1; AC_SUBST([HAVE_MKNOD]) HAVE_MKNODAT=1; AC_SUBST([HAVE_MKNODAT]) HAVE_UTIMENSAT=1; AC_SUBST([HAVE_UTIMENSAT]) REPLACE_FSTAT=0; AC_SUBST([REPLACE_FSTAT]) REPLACE_FSTATAT=0; AC_SUBST([REPLACE_FSTATAT]) REPLACE_FUTIMENS=0; AC_SUBST([REPLACE_FUTIMENS]) REPLACE_LSTAT=0; AC_SUBST([REPLACE_LSTAT]) REPLACE_MKDIR=0; AC_SUBST([REPLACE_MKDIR]) REPLACE_MKFIFO=0; AC_SUBST([REPLACE_MKFIFO]) REPLACE_MKNOD=0; AC_SUBST([REPLACE_MKNOD]) REPLACE_STAT=0; AC_SUBST([REPLACE_STAT]) REPLACE_UTIMENSAT=0; AC_SUBST([REPLACE_UTIMENSAT]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/sys_socket_h.m40000644000175000017500000001416313004436755017116 00000000000000# sys_socket_h.m4 serial 23 dnl Copyright (C) 2005-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Simon Josefsson. AC_DEFUN([gl_HEADER_SYS_SOCKET], [ AC_REQUIRE([gl_SYS_SOCKET_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl On OSF/1, the functions recv(), send(), recvfrom(), sendto() have dnl old-style declarations (with return type 'int' instead of 'ssize_t') dnl unless _POSIX_PII_SOCKET is defined. case "$host_os" in osf*) AC_DEFINE([_POSIX_PII_SOCKET], [1], [Define to 1 in order to get the POSIX compatible declarations of socket functions.]) ;; esac AC_CACHE_CHECK([whether is self-contained], [gl_cv_header_sys_socket_h_selfcontained], [ AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[#include ]], [[]])], [gl_cv_header_sys_socket_h_selfcontained=yes], [gl_cv_header_sys_socket_h_selfcontained=no]) ]) if test $gl_cv_header_sys_socket_h_selfcontained = yes; then dnl If the shutdown function exists, should define dnl SHUT_RD, SHUT_WR, SHUT_RDWR. AC_CHECK_FUNCS([shutdown]) if test $ac_cv_func_shutdown = yes; then AC_CACHE_CHECK([whether defines the SHUT_* macros], [gl_cv_header_sys_socket_h_shut], [ AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include ]], [[int a[] = { SHUT_RD, SHUT_WR, SHUT_RDWR };]])], [gl_cv_header_sys_socket_h_shut=yes], [gl_cv_header_sys_socket_h_shut=no]) ]) if test $gl_cv_header_sys_socket_h_shut = no; then SYS_SOCKET_H='sys/socket.h' fi fi fi # We need to check for ws2tcpip.h now. gl_PREREQ_SYS_H_SOCKET AC_CHECK_TYPES([struct sockaddr_storage, sa_family_t],,,[ /* sys/types.h is not needed according to POSIX, but the sys/socket.h in i386-unknown-freebsd4.10 and powerpc-apple-darwin5.5 required it. */ #include #ifdef HAVE_SYS_SOCKET_H #include #endif #ifdef HAVE_WS2TCPIP_H #include #endif ]) if test $ac_cv_type_struct_sockaddr_storage = no; then HAVE_STRUCT_SOCKADDR_STORAGE=0 fi if test $ac_cv_type_sa_family_t = no; then HAVE_SA_FAMILY_T=0 fi if test $ac_cv_type_struct_sockaddr_storage != no; then AC_CHECK_MEMBERS([struct sockaddr_storage.ss_family], [], [HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY=0], [#include #ifdef HAVE_SYS_SOCKET_H #include #endif #ifdef HAVE_WS2TCPIP_H #include #endif ]) fi if test $HAVE_STRUCT_SOCKADDR_STORAGE = 0 || test $HAVE_SA_FAMILY_T = 0 \ || test $HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = 0; then SYS_SOCKET_H='sys/socket.h' fi gl_PREREQ_SYS_H_WINSOCK2 dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[ /* Some systems require prerequisite headers. */ #include #include ]], [socket connect accept bind getpeername getsockname getsockopt listen recv send recvfrom sendto setsockopt shutdown accept4]) ]) AC_DEFUN([gl_PREREQ_SYS_H_SOCKET], [ dnl Check prerequisites of the replacement. AC_REQUIRE([gl_CHECK_SOCKET_HEADERS]) gl_CHECK_NEXT_HEADERS([sys/socket.h]) if test $ac_cv_header_sys_socket_h = yes; then HAVE_SYS_SOCKET_H=1 HAVE_WS2TCPIP_H=0 else HAVE_SYS_SOCKET_H=0 if test $ac_cv_header_ws2tcpip_h = yes; then HAVE_WS2TCPIP_H=1 else HAVE_WS2TCPIP_H=0 fi fi AC_SUBST([HAVE_SYS_SOCKET_H]) AC_SUBST([HAVE_WS2TCPIP_H]) ]) # Common prerequisites of the replacement and of the # replacement. # Sets and substitutes HAVE_WINSOCK2_H. AC_DEFUN([gl_PREREQ_SYS_H_WINSOCK2], [ m4_ifdef([gl_UNISTD_H_DEFAULTS], [AC_REQUIRE([gl_UNISTD_H_DEFAULTS])]) m4_ifdef([gl_SYS_IOCTL_H_DEFAULTS], [AC_REQUIRE([gl_SYS_IOCTL_H_DEFAULTS])]) AC_CHECK_HEADERS_ONCE([sys/socket.h]) if test $ac_cv_header_sys_socket_h != yes; then dnl We cannot use AC_CHECK_HEADERS_ONCE here, because that would make dnl the check for those headers unconditional; yet cygwin reports dnl that the headers are present but cannot be compiled (since on dnl cygwin, all socket information should come from sys/socket.h). AC_CHECK_HEADERS([winsock2.h]) fi if test "$ac_cv_header_winsock2_h" = yes; then HAVE_WINSOCK2_H=1 UNISTD_H_HAVE_WINSOCK2_H=1 SYS_IOCTL_H_HAVE_WINSOCK2_H=1 else HAVE_WINSOCK2_H=0 fi AC_SUBST([HAVE_WINSOCK2_H]) ]) AC_DEFUN([gl_SYS_SOCKET_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_SYS_SOCKET_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_SYS_SOCKET_H_DEFAULTS], [ GNULIB_SOCKET=0; AC_SUBST([GNULIB_SOCKET]) GNULIB_CONNECT=0; AC_SUBST([GNULIB_CONNECT]) GNULIB_ACCEPT=0; AC_SUBST([GNULIB_ACCEPT]) GNULIB_BIND=0; AC_SUBST([GNULIB_BIND]) GNULIB_GETPEERNAME=0; AC_SUBST([GNULIB_GETPEERNAME]) GNULIB_GETSOCKNAME=0; AC_SUBST([GNULIB_GETSOCKNAME]) GNULIB_GETSOCKOPT=0; AC_SUBST([GNULIB_GETSOCKOPT]) GNULIB_LISTEN=0; AC_SUBST([GNULIB_LISTEN]) GNULIB_RECV=0; AC_SUBST([GNULIB_RECV]) GNULIB_SEND=0; AC_SUBST([GNULIB_SEND]) GNULIB_RECVFROM=0; AC_SUBST([GNULIB_RECVFROM]) GNULIB_SENDTO=0; AC_SUBST([GNULIB_SENDTO]) GNULIB_SETSOCKOPT=0; AC_SUBST([GNULIB_SETSOCKOPT]) GNULIB_SHUTDOWN=0; AC_SUBST([GNULIB_SHUTDOWN]) GNULIB_ACCEPT4=0; AC_SUBST([GNULIB_ACCEPT4]) HAVE_STRUCT_SOCKADDR_STORAGE=1; AC_SUBST([HAVE_STRUCT_SOCKADDR_STORAGE]) HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY=1; AC_SUBST([HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY]) HAVE_SA_FAMILY_T=1; AC_SUBST([HAVE_SA_FAMILY_T]) HAVE_ACCEPT4=1; AC_SUBST([HAVE_ACCEPT4]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/symlink.m40000644000175000017500000000347113004436755016107 00000000000000# serial 6 # See if we need to provide symlink replacement. dnl Copyright (C) 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # Written by Eric Blake. AC_DEFUN([gl_FUNC_SYMLINK], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CHECK_FUNCS_ONCE([symlink]) dnl The best we can do on mingw is provide a dummy that always fails, so dnl that compilation can proceed with fewer ifdefs. On FreeBSD 7.2, AIX 7.1, dnl and Solaris 9, we want to fix a bug with trailing slash handling. if test $ac_cv_func_symlink = no; then HAVE_SYMLINK=0 else AC_CACHE_CHECK([whether symlink handles trailing slash correctly], [gl_cv_func_symlink_works], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[int result = 0; if (!symlink ("a", "conftest.link/")) result |= 1; if (symlink ("conftest.f", "conftest.lnk2")) result |= 2; else if (!symlink ("a", "conftest.lnk2/")) result |= 4; return result; ]])], [gl_cv_func_symlink_works=yes], [gl_cv_func_symlink_works=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_symlink_works="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_symlink_works="guessing no" ;; esac ]) rm -f conftest.f conftest.link conftest.lnk2]) case "$gl_cv_func_symlink_works" in *yes) ;; *) REPLACE_SYMLINK=1 ;; esac fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/strnlen.m40000644000175000017500000000156113004436755016104 00000000000000# strnlen.m4 serial 13 dnl Copyright (C) 2002-2003, 2005-2007, 2009-2016 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_STRNLEN], [ AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) dnl Persuade glibc to declare strnlen(). AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_CHECK_DECLS_ONCE([strnlen]) if test $ac_cv_have_decl_strnlen = no; then HAVE_DECL_STRNLEN=0 else m4_pushdef([AC_LIBOBJ], [:]) dnl Note: AC_FUNC_STRNLEN does AC_LIBOBJ([strnlen]). AC_FUNC_STRNLEN m4_popdef([AC_LIBOBJ]) if test $ac_cv_func_strnlen_working = no; then REPLACE_STRNLEN=1 fi fi ]) # Prerequisites of lib/strnlen.c. AC_DEFUN([gl_PREREQ_STRNLEN], [:]) gnuastro-0.2.33-8a3b/bootstrapped/m4/strndup.m40000644000175000017500000000327413004436755016121 00000000000000# strndup.m4 serial 22 dnl Copyright (C) 2002-2003, 2005-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_STRNDUP], [ dnl Persuade glibc to declare strndup(). AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) AC_CHECK_DECLS_ONCE([strndup]) AC_CHECK_FUNCS_ONCE([strndup]) if test $ac_cv_have_decl_strndup = no; then HAVE_DECL_STRNDUP=0 fi if test $ac_cv_func_strndup = yes; then HAVE_STRNDUP=1 # AIX 4.3.3, AIX 5.1 have a function that fails to add the terminating '\0'. AC_CACHE_CHECK([for working strndup], [gl_cv_func_strndup_works], [AC_RUN_IFELSE([ AC_LANG_PROGRAM([[#include #include ]], [[ #if !HAVE_DECL_STRNDUP extern #ifdef __cplusplus "C" #endif char *strndup (const char *, size_t); #endif int result; char *s; s = strndup ("some longer string", 15); free (s); s = strndup ("shorter string", 13); result = s[13] != '\0'; free (s); return result;]])], [gl_cv_func_strndup_works=yes], [gl_cv_func_strndup_works=no], [ changequote(,)dnl case $host_os in aix | aix[3-6]*) gl_cv_func_strndup_works="guessing no";; *) gl_cv_func_strndup_works="guessing yes";; esac changequote([,])dnl ])]) case $gl_cv_func_strndup_works in *no) REPLACE_STRNDUP=1 ;; esac else HAVE_STRNDUP=0 fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/strings_h.m40000644000175000017500000000316313004436755016417 00000000000000# Configure a replacement for . # serial 6 # Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_HEADER_STRINGS_H], [ dnl Use AC_REQUIRE here, so that the default behavior below is expanded dnl once only, before all statements that occur in other macros. AC_REQUIRE([gl_HEADER_STRINGS_H_BODY]) ]) AC_DEFUN([gl_HEADER_STRINGS_H_BODY], [ AC_REQUIRE([gl_HEADER_STRINGS_H_DEFAULTS]) gl_CHECK_NEXT_HEADERS([strings.h]) if test $ac_cv_header_strings_h = yes; then HAVE_STRINGS_H=1 else HAVE_STRINGS_H=0 fi AC_SUBST([HAVE_STRINGS_H]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[ /* Minix 3.1.8 has a bug: must be included before . */ #include #include ]], [ffs strcasecmp strncasecmp]) ]) AC_DEFUN([gl_STRINGS_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_HEADER_STRINGS_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) ]) AC_DEFUN([gl_HEADER_STRINGS_H_DEFAULTS], [ GNULIB_FFS=0; AC_SUBST([GNULIB_FFS]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_FFS=1; AC_SUBST([HAVE_FFS]) HAVE_STRCASECMP=1; AC_SUBST([HAVE_STRCASECMP]) HAVE_DECL_STRNCASECMP=1; AC_SUBST([HAVE_DECL_STRNCASECMP]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/string_h.m40000644000175000017500000001271413004436755016236 00000000000000# Configure a GNU-like replacement for . # Copyright (C) 2007-2016 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # serial 21 # Written by Paul Eggert. AC_DEFUN([gl_HEADER_STRING_H], [ dnl Use AC_REQUIRE here, so that the default behavior below is expanded dnl once only, before all statements that occur in other macros. AC_REQUIRE([gl_HEADER_STRING_H_BODY]) ]) AC_DEFUN([gl_HEADER_STRING_H_BODY], [ AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) gl_NEXT_HEADERS([string.h]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use, and which is not dnl guaranteed by C89. gl_WARN_ON_USE_PREPARE([[#include ]], [ffsl ffsll memmem mempcpy memrchr rawmemchr stpcpy stpncpy strchrnul strdup strncat strndup strnlen strpbrk strsep strcasestr strtok_r strerror_r strsignal strverscmp]) ]) AC_DEFUN([gl_STRING_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_HEADER_STRING_H_DEFAULTS], [ GNULIB_FFSL=0; AC_SUBST([GNULIB_FFSL]) GNULIB_FFSLL=0; AC_SUBST([GNULIB_FFSLL]) GNULIB_MEMCHR=0; AC_SUBST([GNULIB_MEMCHR]) GNULIB_MEMMEM=0; AC_SUBST([GNULIB_MEMMEM]) GNULIB_MEMPCPY=0; AC_SUBST([GNULIB_MEMPCPY]) GNULIB_MEMRCHR=0; AC_SUBST([GNULIB_MEMRCHR]) GNULIB_RAWMEMCHR=0; AC_SUBST([GNULIB_RAWMEMCHR]) GNULIB_STPCPY=0; AC_SUBST([GNULIB_STPCPY]) GNULIB_STPNCPY=0; AC_SUBST([GNULIB_STPNCPY]) GNULIB_STRCHRNUL=0; AC_SUBST([GNULIB_STRCHRNUL]) GNULIB_STRDUP=0; AC_SUBST([GNULIB_STRDUP]) GNULIB_STRNCAT=0; AC_SUBST([GNULIB_STRNCAT]) GNULIB_STRNDUP=0; AC_SUBST([GNULIB_STRNDUP]) GNULIB_STRNLEN=0; AC_SUBST([GNULIB_STRNLEN]) GNULIB_STRPBRK=0; AC_SUBST([GNULIB_STRPBRK]) GNULIB_STRSEP=0; AC_SUBST([GNULIB_STRSEP]) GNULIB_STRSTR=0; AC_SUBST([GNULIB_STRSTR]) GNULIB_STRCASESTR=0; AC_SUBST([GNULIB_STRCASESTR]) GNULIB_STRTOK_R=0; AC_SUBST([GNULIB_STRTOK_R]) GNULIB_MBSLEN=0; AC_SUBST([GNULIB_MBSLEN]) GNULIB_MBSNLEN=0; AC_SUBST([GNULIB_MBSNLEN]) GNULIB_MBSCHR=0; AC_SUBST([GNULIB_MBSCHR]) GNULIB_MBSRCHR=0; AC_SUBST([GNULIB_MBSRCHR]) GNULIB_MBSSTR=0; AC_SUBST([GNULIB_MBSSTR]) GNULIB_MBSCASECMP=0; AC_SUBST([GNULIB_MBSCASECMP]) GNULIB_MBSNCASECMP=0; AC_SUBST([GNULIB_MBSNCASECMP]) GNULIB_MBSPCASECMP=0; AC_SUBST([GNULIB_MBSPCASECMP]) GNULIB_MBSCASESTR=0; AC_SUBST([GNULIB_MBSCASESTR]) GNULIB_MBSCSPN=0; AC_SUBST([GNULIB_MBSCSPN]) GNULIB_MBSPBRK=0; AC_SUBST([GNULIB_MBSPBRK]) GNULIB_MBSSPN=0; AC_SUBST([GNULIB_MBSSPN]) GNULIB_MBSSEP=0; AC_SUBST([GNULIB_MBSSEP]) GNULIB_MBSTOK_R=0; AC_SUBST([GNULIB_MBSTOK_R]) GNULIB_STRERROR=0; AC_SUBST([GNULIB_STRERROR]) GNULIB_STRERROR_R=0; AC_SUBST([GNULIB_STRERROR_R]) GNULIB_STRSIGNAL=0; AC_SUBST([GNULIB_STRSIGNAL]) GNULIB_STRVERSCMP=0; AC_SUBST([GNULIB_STRVERSCMP]) HAVE_MBSLEN=0; AC_SUBST([HAVE_MBSLEN]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_FFSL=1; AC_SUBST([HAVE_FFSL]) HAVE_FFSLL=1; AC_SUBST([HAVE_FFSLL]) HAVE_MEMCHR=1; AC_SUBST([HAVE_MEMCHR]) HAVE_DECL_MEMMEM=1; AC_SUBST([HAVE_DECL_MEMMEM]) HAVE_MEMPCPY=1; AC_SUBST([HAVE_MEMPCPY]) HAVE_DECL_MEMRCHR=1; AC_SUBST([HAVE_DECL_MEMRCHR]) HAVE_RAWMEMCHR=1; AC_SUBST([HAVE_RAWMEMCHR]) HAVE_STPCPY=1; AC_SUBST([HAVE_STPCPY]) HAVE_STPNCPY=1; AC_SUBST([HAVE_STPNCPY]) HAVE_STRCHRNUL=1; AC_SUBST([HAVE_STRCHRNUL]) HAVE_DECL_STRDUP=1; AC_SUBST([HAVE_DECL_STRDUP]) HAVE_DECL_STRNDUP=1; AC_SUBST([HAVE_DECL_STRNDUP]) HAVE_DECL_STRNLEN=1; AC_SUBST([HAVE_DECL_STRNLEN]) HAVE_STRPBRK=1; AC_SUBST([HAVE_STRPBRK]) HAVE_STRSEP=1; AC_SUBST([HAVE_STRSEP]) HAVE_STRCASESTR=1; AC_SUBST([HAVE_STRCASESTR]) HAVE_DECL_STRTOK_R=1; AC_SUBST([HAVE_DECL_STRTOK_R]) HAVE_DECL_STRERROR_R=1; AC_SUBST([HAVE_DECL_STRERROR_R]) HAVE_DECL_STRSIGNAL=1; AC_SUBST([HAVE_DECL_STRSIGNAL]) HAVE_STRVERSCMP=1; AC_SUBST([HAVE_STRVERSCMP]) REPLACE_MEMCHR=0; AC_SUBST([REPLACE_MEMCHR]) REPLACE_MEMMEM=0; AC_SUBST([REPLACE_MEMMEM]) REPLACE_STPNCPY=0; AC_SUBST([REPLACE_STPNCPY]) REPLACE_STRDUP=0; AC_SUBST([REPLACE_STRDUP]) REPLACE_STRSTR=0; AC_SUBST([REPLACE_STRSTR]) REPLACE_STRCASESTR=0; AC_SUBST([REPLACE_STRCASESTR]) REPLACE_STRCHRNUL=0; AC_SUBST([REPLACE_STRCHRNUL]) REPLACE_STRERROR=0; AC_SUBST([REPLACE_STRERROR]) REPLACE_STRERROR_R=0; AC_SUBST([REPLACE_STRERROR_R]) REPLACE_STRNCAT=0; AC_SUBST([REPLACE_STRNCAT]) REPLACE_STRNDUP=0; AC_SUBST([REPLACE_STRNDUP]) REPLACE_STRNLEN=0; AC_SUBST([REPLACE_STRNLEN]) REPLACE_STRSIGNAL=0; AC_SUBST([REPLACE_STRSIGNAL]) REPLACE_STRTOK_R=0; AC_SUBST([REPLACE_STRTOK_R]) UNDEFINE_STRTOK_R=0; AC_SUBST([UNDEFINE_STRTOK_R]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/strerror.m40000644000175000017500000000623613004436755016305 00000000000000# strerror.m4 serial 17 dnl Copyright (C) 2002, 2007-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_STRERROR], [ AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) AC_REQUIRE([gl_HEADER_ERRNO_H]) AC_REQUIRE([gl_FUNC_STRERROR_0]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles m4_ifdef([gl_FUNC_STRERROR_R_WORKS], [ AC_REQUIRE([gl_FUNC_STRERROR_R_WORKS]) ]) if test "$ERRNO_H:$REPLACE_STRERROR_0" = :0; then AC_CACHE_CHECK([for working strerror function], [gl_cv_func_working_strerror], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[if (!*strerror (-2)) return 1;]])], [gl_cv_func_working_strerror=yes], [gl_cv_func_working_strerror=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_working_strerror="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_working_strerror="guessing no" ;; esac ]) ]) case "$gl_cv_func_working_strerror" in *yes) ;; *) dnl The system's strerror() fails to return a string for out-of-range dnl integers. Replace it. REPLACE_STRERROR=1 ;; esac m4_ifdef([gl_FUNC_STRERROR_R_WORKS], [ dnl If the system's strerror_r or __xpg_strerror_r clobbers strerror's dnl buffer, we must replace strerror. case "$gl_cv_func_strerror_r_works" in *no) REPLACE_STRERROR=1 ;; esac ]) else dnl The system's strerror() cannot know about the new errno values we add dnl to , or any fix for strerror(0). Replace it. REPLACE_STRERROR=1 fi ]) dnl Detect if strerror(0) passes (that is, does not set errno, and does not dnl return a string that matches strerror(-1)). AC_DEFUN([gl_FUNC_STRERROR_0], [ AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles REPLACE_STRERROR_0=0 AC_CACHE_CHECK([whether strerror(0) succeeds], [gl_cv_func_strerror_0_works], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include ]], [[int result = 0; char *str; errno = 0; str = strerror (0); if (!*str) result |= 1; if (errno) result |= 2; if (strstr (str, "nknown") || strstr (str, "ndefined")) result |= 4; return result;]])], [gl_cv_func_strerror_0_works=yes], [gl_cv_func_strerror_0_works=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_strerror_0_works="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_strerror_0_works="guessing no" ;; esac ]) ]) case "$gl_cv_func_strerror_0_works" in *yes) ;; *) REPLACE_STRERROR_0=1 AC_DEFINE([REPLACE_STRERROR_0], [1], [Define to 1 if strerror(0) does not return a message implying success.]) ;; esac ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/strchrnul.m40000644000175000017500000000276613004436755016453 00000000000000# strchrnul.m4 serial 9 dnl Copyright (C) 2003, 2007, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_STRCHRNUL], [ dnl Persuade glibc to declare strchrnul(). AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) AC_CHECK_FUNCS([strchrnul]) if test $ac_cv_func_strchrnul = no; then HAVE_STRCHRNUL=0 else AC_CACHE_CHECK([whether strchrnul works], [gl_cv_func_strchrnul_works], [AC_RUN_IFELSE([AC_LANG_PROGRAM([[ #include /* for strchrnul */ ]], [[const char *buf = "a"; return strchrnul (buf, 'b') != buf + 1; ]])], [gl_cv_func_strchrnul_works=yes], [gl_cv_func_strchrnul_works=no], [dnl Cygwin 1.7.9 introduced strchrnul, but it was broken until 1.7.10 AC_EGREP_CPP([Lucky user], [ #if defined __CYGWIN__ #include #if CYGWIN_VERSION_DLL_COMBINED > CYGWIN_VERSION_DLL_MAKE_COMBINED (1007, 9) Lucky user #endif #else Lucky user #endif ], [gl_cv_func_strchrnul_works="guessing yes"], [gl_cv_func_strchrnul_works="guessing no"]) ]) ]) case "$gl_cv_func_strchrnul_works" in *yes) ;; *) REPLACE_STRCHRNUL=1 ;; esac fi ]) # Prerequisites of lib/strchrnul.c. AC_DEFUN([gl_PREREQ_STRCHRNUL], [:]) gnuastro-0.2.33-8a3b/bootstrapped/m4/strcase.m40000644000175000017500000000201213004436755016053 00000000000000# strcase.m4 serial 11 dnl Copyright (C) 2002, 2005-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_STRCASE], [ gl_FUNC_STRCASECMP gl_FUNC_STRNCASECMP ]) AC_DEFUN([gl_FUNC_STRCASECMP], [ AC_REQUIRE([gl_HEADER_STRINGS_H_DEFAULTS]) AC_CHECK_FUNCS([strcasecmp]) if test $ac_cv_func_strcasecmp = no; then HAVE_STRCASECMP=0 fi ]) AC_DEFUN([gl_FUNC_STRNCASECMP], [ AC_REQUIRE([gl_HEADER_STRINGS_H_DEFAULTS]) AC_CHECK_FUNCS([strncasecmp]) if test $ac_cv_func_strncasecmp = yes; then HAVE_STRNCASECMP=1 else HAVE_STRNCASECMP=0 fi AC_CHECK_DECLS([strncasecmp]) if test $ac_cv_have_decl_strncasecmp = no; then HAVE_DECL_STRNCASECMP=0 fi ]) # Prerequisites of lib/strcasecmp.c. AC_DEFUN([gl_PREREQ_STRCASECMP], [ : ]) # Prerequisites of lib/strncasecmp.c. AC_DEFUN([gl_PREREQ_STRNCASECMP], [ : ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/stdlib_h.m40000644000175000017500000001335513004436755016213 00000000000000# stdlib_h.m4 serial 43 dnl Copyright (C) 2007-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_STDLIB_H], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) gl_NEXT_HEADERS([stdlib.h]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use, and which is not dnl guaranteed by C89. gl_WARN_ON_USE_PREPARE([[#include #if HAVE_SYS_LOADAVG_H # include #endif #if HAVE_RANDOM_H # include #endif ]], [_Exit atoll canonicalize_file_name getloadavg getsubopt grantpt initstate initstate_r mkdtemp mkostemp mkostemps mkstemp mkstemps posix_openpt ptsname ptsname_r qsort_r random random_r realpath rpmatch secure_getenv setenv setstate setstate_r srandom srandom_r strtod strtoll strtoull unlockpt unsetenv]) ]) AC_DEFUN([gl_STDLIB_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_STDLIB_H_DEFAULTS], [ GNULIB__EXIT=0; AC_SUBST([GNULIB__EXIT]) GNULIB_ATOLL=0; AC_SUBST([GNULIB_ATOLL]) GNULIB_CALLOC_POSIX=0; AC_SUBST([GNULIB_CALLOC_POSIX]) GNULIB_CANONICALIZE_FILE_NAME=0; AC_SUBST([GNULIB_CANONICALIZE_FILE_NAME]) GNULIB_GETLOADAVG=0; AC_SUBST([GNULIB_GETLOADAVG]) GNULIB_GETSUBOPT=0; AC_SUBST([GNULIB_GETSUBOPT]) GNULIB_GRANTPT=0; AC_SUBST([GNULIB_GRANTPT]) GNULIB_MALLOC_POSIX=0; AC_SUBST([GNULIB_MALLOC_POSIX]) GNULIB_MBTOWC=0; AC_SUBST([GNULIB_MBTOWC]) GNULIB_MKDTEMP=0; AC_SUBST([GNULIB_MKDTEMP]) GNULIB_MKOSTEMP=0; AC_SUBST([GNULIB_MKOSTEMP]) GNULIB_MKOSTEMPS=0; AC_SUBST([GNULIB_MKOSTEMPS]) GNULIB_MKSTEMP=0; AC_SUBST([GNULIB_MKSTEMP]) GNULIB_MKSTEMPS=0; AC_SUBST([GNULIB_MKSTEMPS]) GNULIB_POSIX_OPENPT=0; AC_SUBST([GNULIB_POSIX_OPENPT]) GNULIB_PTSNAME=0; AC_SUBST([GNULIB_PTSNAME]) GNULIB_PTSNAME_R=0; AC_SUBST([GNULIB_PTSNAME_R]) GNULIB_PUTENV=0; AC_SUBST([GNULIB_PUTENV]) GNULIB_QSORT_R=0; AC_SUBST([GNULIB_QSORT_R]) GNULIB_RANDOM=0; AC_SUBST([GNULIB_RANDOM]) GNULIB_RANDOM_R=0; AC_SUBST([GNULIB_RANDOM_R]) GNULIB_REALLOC_POSIX=0; AC_SUBST([GNULIB_REALLOC_POSIX]) GNULIB_REALPATH=0; AC_SUBST([GNULIB_REALPATH]) GNULIB_RPMATCH=0; AC_SUBST([GNULIB_RPMATCH]) GNULIB_SECURE_GETENV=0; AC_SUBST([GNULIB_SECURE_GETENV]) GNULIB_SETENV=0; AC_SUBST([GNULIB_SETENV]) GNULIB_STRTOD=0; AC_SUBST([GNULIB_STRTOD]) GNULIB_STRTOLL=0; AC_SUBST([GNULIB_STRTOLL]) GNULIB_STRTOULL=0; AC_SUBST([GNULIB_STRTOULL]) GNULIB_SYSTEM_POSIX=0; AC_SUBST([GNULIB_SYSTEM_POSIX]) GNULIB_UNLOCKPT=0; AC_SUBST([GNULIB_UNLOCKPT]) GNULIB_UNSETENV=0; AC_SUBST([GNULIB_UNSETENV]) GNULIB_WCTOMB=0; AC_SUBST([GNULIB_WCTOMB]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE__EXIT=1; AC_SUBST([HAVE__EXIT]) HAVE_ATOLL=1; AC_SUBST([HAVE_ATOLL]) HAVE_CANONICALIZE_FILE_NAME=1; AC_SUBST([HAVE_CANONICALIZE_FILE_NAME]) HAVE_DECL_GETLOADAVG=1; AC_SUBST([HAVE_DECL_GETLOADAVG]) HAVE_GETSUBOPT=1; AC_SUBST([HAVE_GETSUBOPT]) HAVE_GRANTPT=1; AC_SUBST([HAVE_GRANTPT]) HAVE_MKDTEMP=1; AC_SUBST([HAVE_MKDTEMP]) HAVE_MKOSTEMP=1; AC_SUBST([HAVE_MKOSTEMP]) HAVE_MKOSTEMPS=1; AC_SUBST([HAVE_MKOSTEMPS]) HAVE_MKSTEMP=1; AC_SUBST([HAVE_MKSTEMP]) HAVE_MKSTEMPS=1; AC_SUBST([HAVE_MKSTEMPS]) HAVE_POSIX_OPENPT=1; AC_SUBST([HAVE_POSIX_OPENPT]) HAVE_PTSNAME=1; AC_SUBST([HAVE_PTSNAME]) HAVE_PTSNAME_R=1; AC_SUBST([HAVE_PTSNAME_R]) HAVE_QSORT_R=1; AC_SUBST([HAVE_QSORT_R]) HAVE_RANDOM=1; AC_SUBST([HAVE_RANDOM]) HAVE_RANDOM_H=1; AC_SUBST([HAVE_RANDOM_H]) HAVE_RANDOM_R=1; AC_SUBST([HAVE_RANDOM_R]) HAVE_REALPATH=1; AC_SUBST([HAVE_REALPATH]) HAVE_RPMATCH=1; AC_SUBST([HAVE_RPMATCH]) HAVE_SECURE_GETENV=1; AC_SUBST([HAVE_SECURE_GETENV]) HAVE_SETENV=1; AC_SUBST([HAVE_SETENV]) HAVE_DECL_SETENV=1; AC_SUBST([HAVE_DECL_SETENV]) HAVE_STRTOD=1; AC_SUBST([HAVE_STRTOD]) HAVE_STRTOLL=1; AC_SUBST([HAVE_STRTOLL]) HAVE_STRTOULL=1; AC_SUBST([HAVE_STRTOULL]) HAVE_STRUCT_RANDOM_DATA=1; AC_SUBST([HAVE_STRUCT_RANDOM_DATA]) HAVE_SYS_LOADAVG_H=0; AC_SUBST([HAVE_SYS_LOADAVG_H]) HAVE_UNLOCKPT=1; AC_SUBST([HAVE_UNLOCKPT]) HAVE_DECL_UNSETENV=1; AC_SUBST([HAVE_DECL_UNSETENV]) REPLACE_CALLOC=0; AC_SUBST([REPLACE_CALLOC]) REPLACE_CANONICALIZE_FILE_NAME=0; AC_SUBST([REPLACE_CANONICALIZE_FILE_NAME]) REPLACE_MALLOC=0; AC_SUBST([REPLACE_MALLOC]) REPLACE_MBTOWC=0; AC_SUBST([REPLACE_MBTOWC]) REPLACE_MKSTEMP=0; AC_SUBST([REPLACE_MKSTEMP]) REPLACE_PTSNAME=0; AC_SUBST([REPLACE_PTSNAME]) REPLACE_PTSNAME_R=0; AC_SUBST([REPLACE_PTSNAME_R]) REPLACE_PUTENV=0; AC_SUBST([REPLACE_PUTENV]) REPLACE_QSORT_R=0; AC_SUBST([REPLACE_QSORT_R]) REPLACE_RANDOM_R=0; AC_SUBST([REPLACE_RANDOM_R]) REPLACE_REALLOC=0; AC_SUBST([REPLACE_REALLOC]) REPLACE_REALPATH=0; AC_SUBST([REPLACE_REALPATH]) REPLACE_SETENV=0; AC_SUBST([REPLACE_SETENV]) REPLACE_STRTOD=0; AC_SUBST([REPLACE_STRTOD]) REPLACE_UNSETENV=0; AC_SUBST([REPLACE_UNSETENV]) REPLACE_WCTOMB=0; AC_SUBST([REPLACE_WCTOMB]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/stdio_h.m40000644000175000017500000002525613004436755016057 00000000000000# stdio_h.m4 serial 48 dnl Copyright (C) 2007-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_STDIO_H], [ AH_VERBATIM([MINGW_ANSI_STDIO], [/* Use GNU style printf and scanf. */ #ifndef __USE_MINGW_ANSI_STDIO # undef __USE_MINGW_ANSI_STDIO #endif ]) AC_DEFINE([__USE_MINGW_ANSI_STDIO]) AC_REQUIRE([gl_STDIO_H_DEFAULTS]) gl_NEXT_HEADERS([stdio.h]) dnl Determine whether __USE_MINGW_ANSI_STDIO makes printf and dnl inttypes.h behave like gnu instead of system; we must give our dnl printf wrapper the right attribute to match. AC_CACHE_CHECK([which flavor of printf attribute matches inttypes macros], [gl_cv_func_printf_attribute_flavor], [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[ #define __STDC_FORMAT_MACROS 1 #include #include /* For non-mingw systems, compilation will trivially succeed. For mingw, compilation will succeed for older mingw (system printf, "I64d") and fail for newer mingw (gnu printf, "lld"). */ #if ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) && \ (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) extern char PRIdMAX_probe[sizeof PRIdMAX == sizeof "I64d" ? 1 : -1]; #endif ]])], [gl_cv_func_printf_attribute_flavor=system], [gl_cv_func_printf_attribute_flavor=gnu])]) if test "$gl_cv_func_printf_attribute_flavor" = gnu; then AC_DEFINE([GNULIB_PRINTF_ATTRIBUTE_FLAVOR_GNU], [1], [Define to 1 if printf and friends should be labeled with attribute "__gnu_printf__" instead of "__printf__"]) fi dnl No need to create extra modules for these functions. Everyone who uses dnl likely needs them. GNULIB_FSCANF=1 gl_MODULE_INDICATOR([fscanf]) GNULIB_SCANF=1 gl_MODULE_INDICATOR([scanf]) GNULIB_FGETC=1 GNULIB_GETC=1 GNULIB_GETCHAR=1 GNULIB_FGETS=1 GNULIB_FREAD=1 dnl This ifdef is necessary to avoid an error "missing file lib/stdio-read.c" dnl "expected source file, required through AC_LIBSOURCES, not found". It is dnl also an optimization, to avoid performing a configure check whose result dnl is not used. But it does not make the test of GNULIB_STDIO_H_NONBLOCKING dnl or GNULIB_NONBLOCKING redundant. m4_ifdef([gl_NONBLOCKING_IO], [ gl_NONBLOCKING_IO if test $gl_cv_have_nonblocking != yes; then REPLACE_STDIO_READ_FUNCS=1 AC_LIBOBJ([stdio-read]) fi ]) dnl No need to create extra modules for these functions. Everyone who uses dnl likely needs them. GNULIB_FPRINTF=1 GNULIB_PRINTF=1 GNULIB_VFPRINTF=1 GNULIB_VPRINTF=1 GNULIB_FPUTC=1 GNULIB_PUTC=1 GNULIB_PUTCHAR=1 GNULIB_FPUTS=1 GNULIB_PUTS=1 GNULIB_FWRITE=1 dnl This ifdef is necessary to avoid an error "missing file lib/stdio-write.c" dnl "expected source file, required through AC_LIBSOURCES, not found". It is dnl also an optimization, to avoid performing a configure check whose result dnl is not used. But it does not make the test of GNULIB_STDIO_H_SIGPIPE or dnl GNULIB_SIGPIPE redundant. m4_ifdef([gl_SIGNAL_SIGPIPE], [ gl_SIGNAL_SIGPIPE if test $gl_cv_header_signal_h_SIGPIPE != yes; then REPLACE_STDIO_WRITE_FUNCS=1 AC_LIBOBJ([stdio-write]) fi ]) dnl This ifdef is necessary to avoid an error "missing file lib/stdio-write.c" dnl "expected source file, required through AC_LIBSOURCES, not found". It is dnl also an optimization, to avoid performing a configure check whose result dnl is not used. But it does not make the test of GNULIB_STDIO_H_NONBLOCKING dnl or GNULIB_NONBLOCKING redundant. m4_ifdef([gl_NONBLOCKING_IO], [ gl_NONBLOCKING_IO if test $gl_cv_have_nonblocking != yes; then REPLACE_STDIO_WRITE_FUNCS=1 AC_LIBOBJ([stdio-write]) fi ]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use, and which is not dnl guaranteed by both C89 and C11. gl_WARN_ON_USE_PREPARE([[#include ]], [dprintf fpurge fseeko ftello getdelim getline gets pclose popen renameat snprintf tmpfile vdprintf vsnprintf]) ]) AC_DEFUN([gl_STDIO_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_STDIO_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_STDIO_H_DEFAULTS], [ GNULIB_DPRINTF=0; AC_SUBST([GNULIB_DPRINTF]) GNULIB_FCLOSE=0; AC_SUBST([GNULIB_FCLOSE]) GNULIB_FDOPEN=0; AC_SUBST([GNULIB_FDOPEN]) GNULIB_FFLUSH=0; AC_SUBST([GNULIB_FFLUSH]) GNULIB_FGETC=0; AC_SUBST([GNULIB_FGETC]) GNULIB_FGETS=0; AC_SUBST([GNULIB_FGETS]) GNULIB_FOPEN=0; AC_SUBST([GNULIB_FOPEN]) GNULIB_FPRINTF=0; AC_SUBST([GNULIB_FPRINTF]) GNULIB_FPRINTF_POSIX=0; AC_SUBST([GNULIB_FPRINTF_POSIX]) GNULIB_FPURGE=0; AC_SUBST([GNULIB_FPURGE]) GNULIB_FPUTC=0; AC_SUBST([GNULIB_FPUTC]) GNULIB_FPUTS=0; AC_SUBST([GNULIB_FPUTS]) GNULIB_FREAD=0; AC_SUBST([GNULIB_FREAD]) GNULIB_FREOPEN=0; AC_SUBST([GNULIB_FREOPEN]) GNULIB_FSCANF=0; AC_SUBST([GNULIB_FSCANF]) GNULIB_FSEEK=0; AC_SUBST([GNULIB_FSEEK]) GNULIB_FSEEKO=0; AC_SUBST([GNULIB_FSEEKO]) GNULIB_FTELL=0; AC_SUBST([GNULIB_FTELL]) GNULIB_FTELLO=0; AC_SUBST([GNULIB_FTELLO]) GNULIB_FWRITE=0; AC_SUBST([GNULIB_FWRITE]) GNULIB_GETC=0; AC_SUBST([GNULIB_GETC]) GNULIB_GETCHAR=0; AC_SUBST([GNULIB_GETCHAR]) GNULIB_GETDELIM=0; AC_SUBST([GNULIB_GETDELIM]) GNULIB_GETLINE=0; AC_SUBST([GNULIB_GETLINE]) GNULIB_OBSTACK_PRINTF=0; AC_SUBST([GNULIB_OBSTACK_PRINTF]) GNULIB_OBSTACK_PRINTF_POSIX=0; AC_SUBST([GNULIB_OBSTACK_PRINTF_POSIX]) GNULIB_PCLOSE=0; AC_SUBST([GNULIB_PCLOSE]) GNULIB_PERROR=0; AC_SUBST([GNULIB_PERROR]) GNULIB_POPEN=0; AC_SUBST([GNULIB_POPEN]) GNULIB_PRINTF=0; AC_SUBST([GNULIB_PRINTF]) GNULIB_PRINTF_POSIX=0; AC_SUBST([GNULIB_PRINTF_POSIX]) GNULIB_PUTC=0; AC_SUBST([GNULIB_PUTC]) GNULIB_PUTCHAR=0; AC_SUBST([GNULIB_PUTCHAR]) GNULIB_PUTS=0; AC_SUBST([GNULIB_PUTS]) GNULIB_REMOVE=0; AC_SUBST([GNULIB_REMOVE]) GNULIB_RENAME=0; AC_SUBST([GNULIB_RENAME]) GNULIB_RENAMEAT=0; AC_SUBST([GNULIB_RENAMEAT]) GNULIB_SCANF=0; AC_SUBST([GNULIB_SCANF]) GNULIB_SNPRINTF=0; AC_SUBST([GNULIB_SNPRINTF]) GNULIB_SPRINTF_POSIX=0; AC_SUBST([GNULIB_SPRINTF_POSIX]) GNULIB_STDIO_H_NONBLOCKING=0; AC_SUBST([GNULIB_STDIO_H_NONBLOCKING]) GNULIB_STDIO_H_SIGPIPE=0; AC_SUBST([GNULIB_STDIO_H_SIGPIPE]) GNULIB_TMPFILE=0; AC_SUBST([GNULIB_TMPFILE]) GNULIB_VASPRINTF=0; AC_SUBST([GNULIB_VASPRINTF]) GNULIB_VFSCANF=0; AC_SUBST([GNULIB_VFSCANF]) GNULIB_VSCANF=0; AC_SUBST([GNULIB_VSCANF]) GNULIB_VDPRINTF=0; AC_SUBST([GNULIB_VDPRINTF]) GNULIB_VFPRINTF=0; AC_SUBST([GNULIB_VFPRINTF]) GNULIB_VFPRINTF_POSIX=0; AC_SUBST([GNULIB_VFPRINTF_POSIX]) GNULIB_VPRINTF=0; AC_SUBST([GNULIB_VPRINTF]) GNULIB_VPRINTF_POSIX=0; AC_SUBST([GNULIB_VPRINTF_POSIX]) GNULIB_VSNPRINTF=0; AC_SUBST([GNULIB_VSNPRINTF]) GNULIB_VSPRINTF_POSIX=0; AC_SUBST([GNULIB_VSPRINTF_POSIX]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_DECL_FPURGE=1; AC_SUBST([HAVE_DECL_FPURGE]) HAVE_DECL_FSEEKO=1; AC_SUBST([HAVE_DECL_FSEEKO]) HAVE_DECL_FTELLO=1; AC_SUBST([HAVE_DECL_FTELLO]) HAVE_DECL_GETDELIM=1; AC_SUBST([HAVE_DECL_GETDELIM]) HAVE_DECL_GETLINE=1; AC_SUBST([HAVE_DECL_GETLINE]) HAVE_DECL_OBSTACK_PRINTF=1; AC_SUBST([HAVE_DECL_OBSTACK_PRINTF]) HAVE_DECL_SNPRINTF=1; AC_SUBST([HAVE_DECL_SNPRINTF]) HAVE_DECL_VSNPRINTF=1; AC_SUBST([HAVE_DECL_VSNPRINTF]) HAVE_DPRINTF=1; AC_SUBST([HAVE_DPRINTF]) HAVE_FSEEKO=1; AC_SUBST([HAVE_FSEEKO]) HAVE_FTELLO=1; AC_SUBST([HAVE_FTELLO]) HAVE_PCLOSE=1; AC_SUBST([HAVE_PCLOSE]) HAVE_POPEN=1; AC_SUBST([HAVE_POPEN]) HAVE_RENAMEAT=1; AC_SUBST([HAVE_RENAMEAT]) HAVE_VASPRINTF=1; AC_SUBST([HAVE_VASPRINTF]) HAVE_VDPRINTF=1; AC_SUBST([HAVE_VDPRINTF]) REPLACE_DPRINTF=0; AC_SUBST([REPLACE_DPRINTF]) REPLACE_FCLOSE=0; AC_SUBST([REPLACE_FCLOSE]) REPLACE_FDOPEN=0; AC_SUBST([REPLACE_FDOPEN]) REPLACE_FFLUSH=0; AC_SUBST([REPLACE_FFLUSH]) REPLACE_FOPEN=0; AC_SUBST([REPLACE_FOPEN]) REPLACE_FPRINTF=0; AC_SUBST([REPLACE_FPRINTF]) REPLACE_FPURGE=0; AC_SUBST([REPLACE_FPURGE]) REPLACE_FREOPEN=0; AC_SUBST([REPLACE_FREOPEN]) REPLACE_FSEEK=0; AC_SUBST([REPLACE_FSEEK]) REPLACE_FSEEKO=0; AC_SUBST([REPLACE_FSEEKO]) REPLACE_FTELL=0; AC_SUBST([REPLACE_FTELL]) REPLACE_FTELLO=0; AC_SUBST([REPLACE_FTELLO]) REPLACE_GETDELIM=0; AC_SUBST([REPLACE_GETDELIM]) REPLACE_GETLINE=0; AC_SUBST([REPLACE_GETLINE]) REPLACE_OBSTACK_PRINTF=0; AC_SUBST([REPLACE_OBSTACK_PRINTF]) REPLACE_PERROR=0; AC_SUBST([REPLACE_PERROR]) REPLACE_POPEN=0; AC_SUBST([REPLACE_POPEN]) REPLACE_PRINTF=0; AC_SUBST([REPLACE_PRINTF]) REPLACE_REMOVE=0; AC_SUBST([REPLACE_REMOVE]) REPLACE_RENAME=0; AC_SUBST([REPLACE_RENAME]) REPLACE_RENAMEAT=0; AC_SUBST([REPLACE_RENAMEAT]) REPLACE_SNPRINTF=0; AC_SUBST([REPLACE_SNPRINTF]) REPLACE_SPRINTF=0; AC_SUBST([REPLACE_SPRINTF]) REPLACE_STDIO_READ_FUNCS=0; AC_SUBST([REPLACE_STDIO_READ_FUNCS]) REPLACE_STDIO_WRITE_FUNCS=0; AC_SUBST([REPLACE_STDIO_WRITE_FUNCS]) REPLACE_TMPFILE=0; AC_SUBST([REPLACE_TMPFILE]) REPLACE_VASPRINTF=0; AC_SUBST([REPLACE_VASPRINTF]) REPLACE_VDPRINTF=0; AC_SUBST([REPLACE_VDPRINTF]) REPLACE_VFPRINTF=0; AC_SUBST([REPLACE_VFPRINTF]) REPLACE_VPRINTF=0; AC_SUBST([REPLACE_VPRINTF]) REPLACE_VSNPRINTF=0; AC_SUBST([REPLACE_VSNPRINTF]) REPLACE_VSPRINTF=0; AC_SUBST([REPLACE_VSPRINTF]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/stdint_h.m40000644000175000017500000000174313004436755016235 00000000000000# stdint_h.m4 serial 9 dnl Copyright (C) 1997-2004, 2006, 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Paul Eggert. # Define HAVE_STDINT_H_WITH_UINTMAX if exists, # doesn't clash with , and declares uintmax_t. AC_DEFUN([gl_AC_HEADER_STDINT_H], [ AC_CACHE_CHECK([for stdint.h], [gl_cv_header_stdint_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include #include ]], [[uintmax_t i = (uintmax_t) -1; return !i;]])], [gl_cv_header_stdint_h=yes], [gl_cv_header_stdint_h=no])]) if test $gl_cv_header_stdint_h = yes; then AC_DEFINE_UNQUOTED([HAVE_STDINT_H_WITH_UINTMAX], [1], [Define if exists, doesn't clash with , and declares uintmax_t. ]) fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/stdint.m40000644000175000017500000004311013004436755015720 00000000000000# stdint.m4 serial 48 dnl Copyright (C) 2001-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Paul Eggert and Bruno Haible. dnl Test whether is supported or must be substituted. AC_DEFUN_ONCE([gl_STDINT_H], [ AC_PREREQ([2.59])dnl AC_REQUIRE([gl_LIMITS_H]) dnl Check for long long int and unsigned long long int. AC_REQUIRE([AC_TYPE_LONG_LONG_INT]) if test $ac_cv_type_long_long_int = yes; then HAVE_LONG_LONG_INT=1 else HAVE_LONG_LONG_INT=0 fi AC_SUBST([HAVE_LONG_LONG_INT]) AC_REQUIRE([AC_TYPE_UNSIGNED_LONG_LONG_INT]) if test $ac_cv_type_unsigned_long_long_int = yes; then HAVE_UNSIGNED_LONG_LONG_INT=1 else HAVE_UNSIGNED_LONG_LONG_INT=0 fi AC_SUBST([HAVE_UNSIGNED_LONG_LONG_INT]) dnl Check for , in the same way as gl_WCHAR_H does. AC_CHECK_HEADERS_ONCE([wchar.h]) if test $ac_cv_header_wchar_h = yes; then HAVE_WCHAR_H=1 else HAVE_WCHAR_H=0 fi AC_SUBST([HAVE_WCHAR_H]) dnl Check for . dnl AC_INCLUDES_DEFAULT defines $ac_cv_header_inttypes_h. if test $ac_cv_header_inttypes_h = yes; then HAVE_INTTYPES_H=1 else HAVE_INTTYPES_H=0 fi AC_SUBST([HAVE_INTTYPES_H]) dnl Check for . dnl AC_INCLUDES_DEFAULT defines $ac_cv_header_sys_types_h. if test $ac_cv_header_sys_types_h = yes; then HAVE_SYS_TYPES_H=1 else HAVE_SYS_TYPES_H=0 fi AC_SUBST([HAVE_SYS_TYPES_H]) gl_CHECK_NEXT_HEADERS([stdint.h]) if test $ac_cv_header_stdint_h = yes; then HAVE_STDINT_H=1 else HAVE_STDINT_H=0 fi AC_SUBST([HAVE_STDINT_H]) dnl Now see whether we need a substitute . if test $ac_cv_header_stdint_h = yes; then AC_CACHE_CHECK([whether stdint.h conforms to C99], [gl_cv_header_working_stdint_h], [gl_cv_header_working_stdint_h=no AC_COMPILE_IFELSE([ AC_LANG_PROGRAM([[ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 /* work if build isn't clean */ #define __STDC_CONSTANT_MACROS 1 #define __STDC_LIMIT_MACROS 1 #include /* Dragonfly defines WCHAR_MIN, WCHAR_MAX only in . */ #if !(defined WCHAR_MIN && defined WCHAR_MAX) #error "WCHAR_MIN, WCHAR_MAX not defined in " #endif ] gl_STDINT_INCLUDES [ #ifdef INT8_MAX int8_t a1 = INT8_MAX; int8_t a1min = INT8_MIN; #endif #ifdef INT16_MAX int16_t a2 = INT16_MAX; int16_t a2min = INT16_MIN; #endif #ifdef INT32_MAX int32_t a3 = INT32_MAX; int32_t a3min = INT32_MIN; #endif #ifdef INT64_MAX int64_t a4 = INT64_MAX; int64_t a4min = INT64_MIN; #endif #ifdef UINT8_MAX uint8_t b1 = UINT8_MAX; #else typedef int b1[(unsigned char) -1 != 255 ? 1 : -1]; #endif #ifdef UINT16_MAX uint16_t b2 = UINT16_MAX; #endif #ifdef UINT32_MAX uint32_t b3 = UINT32_MAX; #endif #ifdef UINT64_MAX uint64_t b4 = UINT64_MAX; #endif int_least8_t c1 = INT8_C (0x7f); int_least8_t c1max = INT_LEAST8_MAX; int_least8_t c1min = INT_LEAST8_MIN; int_least16_t c2 = INT16_C (0x7fff); int_least16_t c2max = INT_LEAST16_MAX; int_least16_t c2min = INT_LEAST16_MIN; int_least32_t c3 = INT32_C (0x7fffffff); int_least32_t c3max = INT_LEAST32_MAX; int_least32_t c3min = INT_LEAST32_MIN; int_least64_t c4 = INT64_C (0x7fffffffffffffff); int_least64_t c4max = INT_LEAST64_MAX; int_least64_t c4min = INT_LEAST64_MIN; uint_least8_t d1 = UINT8_C (0xff); uint_least8_t d1max = UINT_LEAST8_MAX; uint_least16_t d2 = UINT16_C (0xffff); uint_least16_t d2max = UINT_LEAST16_MAX; uint_least32_t d3 = UINT32_C (0xffffffff); uint_least32_t d3max = UINT_LEAST32_MAX; uint_least64_t d4 = UINT64_C (0xffffffffffffffff); uint_least64_t d4max = UINT_LEAST64_MAX; int_fast8_t e1 = INT_FAST8_MAX; int_fast8_t e1min = INT_FAST8_MIN; int_fast16_t e2 = INT_FAST16_MAX; int_fast16_t e2min = INT_FAST16_MIN; int_fast32_t e3 = INT_FAST32_MAX; int_fast32_t e3min = INT_FAST32_MIN; int_fast64_t e4 = INT_FAST64_MAX; int_fast64_t e4min = INT_FAST64_MIN; uint_fast8_t f1 = UINT_FAST8_MAX; uint_fast16_t f2 = UINT_FAST16_MAX; uint_fast32_t f3 = UINT_FAST32_MAX; uint_fast64_t f4 = UINT_FAST64_MAX; #ifdef INTPTR_MAX intptr_t g = INTPTR_MAX; intptr_t gmin = INTPTR_MIN; #endif #ifdef UINTPTR_MAX uintptr_t h = UINTPTR_MAX; #endif intmax_t i = INTMAX_MAX; uintmax_t j = UINTMAX_MAX; /* Check that SIZE_MAX has the correct type, if possible. */ #if 201112 <= __STDC_VERSION__ int k = _Generic (SIZE_MAX, size_t: 0); #elif (2 <= __GNUC__ || defined __IBM__TYPEOF__ \ || (0x5110 <= __SUNPRO_C && !__STDC__)) extern size_t k; extern __typeof__ (SIZE_MAX) k; #endif #include /* for CHAR_BIT */ #define TYPE_MINIMUM(t) \ ((t) ((t) 0 < (t) -1 ? (t) 0 : ~ TYPE_MAXIMUM (t))) #define TYPE_MAXIMUM(t) \ ((t) ((t) 0 < (t) -1 \ ? (t) -1 \ : ((((t) 1 << (sizeof (t) * CHAR_BIT - 2)) - 1) * 2 + 1))) struct s { int check_PTRDIFF: PTRDIFF_MIN == TYPE_MINIMUM (ptrdiff_t) && PTRDIFF_MAX == TYPE_MAXIMUM (ptrdiff_t) ? 1 : -1; /* Detect bug in FreeBSD 6.0 / ia64. */ int check_SIG_ATOMIC: SIG_ATOMIC_MIN == TYPE_MINIMUM (sig_atomic_t) && SIG_ATOMIC_MAX == TYPE_MAXIMUM (sig_atomic_t) ? 1 : -1; int check_SIZE: SIZE_MAX == TYPE_MAXIMUM (size_t) ? 1 : -1; int check_WCHAR: WCHAR_MIN == TYPE_MINIMUM (wchar_t) && WCHAR_MAX == TYPE_MAXIMUM (wchar_t) ? 1 : -1; /* Detect bug in mingw. */ int check_WINT: WINT_MIN == TYPE_MINIMUM (wint_t) && WINT_MAX == TYPE_MAXIMUM (wint_t) ? 1 : -1; /* Detect bugs in glibc 2.4 and Solaris 10 stdint.h, among others. */ int check_UINT8_C: (-1 < UINT8_C (0)) == (-1 < (uint_least8_t) 0) ? 1 : -1; int check_UINT16_C: (-1 < UINT16_C (0)) == (-1 < (uint_least16_t) 0) ? 1 : -1; /* Detect bugs in OpenBSD 3.9 stdint.h. */ #ifdef UINT8_MAX int check_uint8: (uint8_t) -1 == UINT8_MAX ? 1 : -1; #endif #ifdef UINT16_MAX int check_uint16: (uint16_t) -1 == UINT16_MAX ? 1 : -1; #endif #ifdef UINT32_MAX int check_uint32: (uint32_t) -1 == UINT32_MAX ? 1 : -1; #endif #ifdef UINT64_MAX int check_uint64: (uint64_t) -1 == UINT64_MAX ? 1 : -1; #endif int check_uint_least8: (uint_least8_t) -1 == UINT_LEAST8_MAX ? 1 : -1; int check_uint_least16: (uint_least16_t) -1 == UINT_LEAST16_MAX ? 1 : -1; int check_uint_least32: (uint_least32_t) -1 == UINT_LEAST32_MAX ? 1 : -1; int check_uint_least64: (uint_least64_t) -1 == UINT_LEAST64_MAX ? 1 : -1; int check_uint_fast8: (uint_fast8_t) -1 == UINT_FAST8_MAX ? 1 : -1; int check_uint_fast16: (uint_fast16_t) -1 == UINT_FAST16_MAX ? 1 : -1; int check_uint_fast32: (uint_fast32_t) -1 == UINT_FAST32_MAX ? 1 : -1; int check_uint_fast64: (uint_fast64_t) -1 == UINT_FAST64_MAX ? 1 : -1; int check_uintptr: (uintptr_t) -1 == UINTPTR_MAX ? 1 : -1; int check_uintmax: (uintmax_t) -1 == UINTMAX_MAX ? 1 : -1; int check_size: (size_t) -1 == SIZE_MAX ? 1 : -1; }; ]])], [dnl Determine whether the various *_MIN, *_MAX macros are usable dnl in preprocessor expression. We could do it by compiling a test dnl program for each of these macros. It is faster to run a program dnl that inspects the macro expansion. dnl This detects a bug on HP-UX 11.23/ia64. AC_RUN_IFELSE([ AC_LANG_PROGRAM([[ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 /* work if build isn't clean */ #define __STDC_CONSTANT_MACROS 1 #define __STDC_LIMIT_MACROS 1 #include ] gl_STDINT_INCLUDES [ #include #include #define MVAL(macro) MVAL1(macro) #define MVAL1(expression) #expression static const char *macro_values[] = { #ifdef INT8_MAX MVAL (INT8_MAX), #endif #ifdef INT16_MAX MVAL (INT16_MAX), #endif #ifdef INT32_MAX MVAL (INT32_MAX), #endif #ifdef INT64_MAX MVAL (INT64_MAX), #endif #ifdef UINT8_MAX MVAL (UINT8_MAX), #endif #ifdef UINT16_MAX MVAL (UINT16_MAX), #endif #ifdef UINT32_MAX MVAL (UINT32_MAX), #endif #ifdef UINT64_MAX MVAL (UINT64_MAX), #endif NULL }; ]], [[ const char **mv; for (mv = macro_values; *mv != NULL; mv++) { const char *value = *mv; /* Test whether it looks like a cast expression. */ if (strncmp (value, "((unsigned int)"/*)*/, 15) == 0 || strncmp (value, "((unsigned short)"/*)*/, 17) == 0 || strncmp (value, "((unsigned char)"/*)*/, 16) == 0 || strncmp (value, "((int)"/*)*/, 6) == 0 || strncmp (value, "((signed short)"/*)*/, 15) == 0 || strncmp (value, "((signed char)"/*)*/, 14) == 0) return mv - macro_values + 1; } return 0; ]])], [gl_cv_header_working_stdint_h=yes], [], [dnl When cross-compiling, assume it works. gl_cv_header_working_stdint_h=yes ]) ]) ]) fi HAVE_C99_STDINT_H=0 HAVE_SYS_BITYPES_H=0 HAVE_SYS_INTTYPES_H=0 STDINT_H=stdint.h if test "$gl_cv_header_working_stdint_h" = yes; then HAVE_C99_STDINT_H=1 dnl Now see whether the system works without dnl __STDC_CONSTANT_MACROS/__STDC_LIMIT_MACROS defined. AC_CACHE_CHECK([whether stdint.h predates C++11], [gl_cv_header_stdint_predates_cxx11_h], [gl_cv_header_stdint_predates_cxx11_h=yes AC_COMPILE_IFELSE([ AC_LANG_PROGRAM([[ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 /* work if build isn't clean */ #include ] gl_STDINT_INCLUDES [ intmax_t im = INTMAX_MAX; int32_t i32 = INT32_C (0x7fffffff); ]])], [gl_cv_header_stdint_predates_cxx11_h=no])]) if test "$gl_cv_header_stdint_predates_cxx11_h" = yes; then AC_DEFINE([__STDC_CONSTANT_MACROS], [1], [Define to 1 if the system predates C++11.]) AC_DEFINE([__STDC_LIMIT_MACROS], [1], [Define to 1 if the system predates C++11.]) fi AC_CACHE_CHECK([whether stdint.h has UINTMAX_WIDTH etc.], [gl_cv_header_stdint_width], [gl_cv_header_stdint_width=no AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[ /* Work if build is not clean. */ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 #ifndef __STDC_WANT_IEC_60559_BFP_EXT__ #define __STDC_WANT_IEC_60559_BFP_EXT__ 1 #endif #include ]gl_STDINT_INCLUDES[ int iw = UINTMAX_WIDTH; ]])], [gl_cv_header_stdint_width=yes])]) if test "$gl_cv_header_stdint_width" = yes; then STDINT_H= fi else dnl Check for , and for dnl (used in Linux libc4 >= 4.6.7 and libc5). AC_CHECK_HEADERS([sys/inttypes.h sys/bitypes.h]) if test $ac_cv_header_sys_inttypes_h = yes; then HAVE_SYS_INTTYPES_H=1 fi if test $ac_cv_header_sys_bitypes_h = yes; then HAVE_SYS_BITYPES_H=1 fi gl_STDINT_TYPE_PROPERTIES fi # The substitute stdint.h needs the substitute limit.h's _GL_INTEGER_WIDTH. LIMITS_H=limits.h AM_CONDITIONAL([GL_GENERATE_LIMITS_H], [test -n "$LIMITS_H"]) AC_SUBST([HAVE_C99_STDINT_H]) AC_SUBST([HAVE_SYS_BITYPES_H]) AC_SUBST([HAVE_SYS_INTTYPES_H]) AC_SUBST([STDINT_H]) AM_CONDITIONAL([GL_GENERATE_STDINT_H], [test -n "$STDINT_H"]) ]) dnl gl_STDINT_BITSIZEOF(TYPES, INCLUDES) dnl Determine the size of each of the given types in bits. AC_DEFUN([gl_STDINT_BITSIZEOF], [ dnl Use a shell loop, to avoid bloating configure, and dnl - extra AH_TEMPLATE calls, so that autoheader knows what to put into dnl config.h.in, dnl - extra AC_SUBST calls, so that the right substitutions are made. m4_foreach_w([gltype], [$1], [AH_TEMPLATE([BITSIZEOF_]m4_translit(gltype,[abcdefghijklmnopqrstuvwxyz ],[ABCDEFGHIJKLMNOPQRSTUVWXYZ_]), [Define to the number of bits in type ']gltype['.])]) for gltype in $1 ; do AC_CACHE_CHECK([for bit size of $gltype], [gl_cv_bitsizeof_${gltype}], [AC_COMPUTE_INT([result], [sizeof ($gltype) * CHAR_BIT], [$2 #include ], [result=unknown]) eval gl_cv_bitsizeof_${gltype}=\$result ]) eval result=\$gl_cv_bitsizeof_${gltype} if test $result = unknown; then dnl Use a nonempty default, because some compilers, such as IRIX 5 cc, dnl do a syntax check even on unused #if conditions and give an error dnl on valid C code like this: dnl #if 0 dnl # if > 32 dnl # endif dnl #endif result=0 fi GLTYPE=`echo "$gltype" | tr 'abcdefghijklmnopqrstuvwxyz ' 'ABCDEFGHIJKLMNOPQRSTUVWXYZ_'` AC_DEFINE_UNQUOTED([BITSIZEOF_${GLTYPE}], [$result]) eval BITSIZEOF_${GLTYPE}=\$result done m4_foreach_w([gltype], [$1], [AC_SUBST([BITSIZEOF_]m4_translit(gltype,[abcdefghijklmnopqrstuvwxyz ],[ABCDEFGHIJKLMNOPQRSTUVWXYZ_]))]) ]) dnl gl_CHECK_TYPES_SIGNED(TYPES, INCLUDES) dnl Determine the signedness of each of the given types. dnl Define HAVE_SIGNED_TYPE if type is signed. AC_DEFUN([gl_CHECK_TYPES_SIGNED], [ dnl Use a shell loop, to avoid bloating configure, and dnl - extra AH_TEMPLATE calls, so that autoheader knows what to put into dnl config.h.in, dnl - extra AC_SUBST calls, so that the right substitutions are made. m4_foreach_w([gltype], [$1], [AH_TEMPLATE([HAVE_SIGNED_]m4_translit(gltype,[abcdefghijklmnopqrstuvwxyz ],[ABCDEFGHIJKLMNOPQRSTUVWXYZ_]), [Define to 1 if ']gltype[' is a signed integer type.])]) for gltype in $1 ; do AC_CACHE_CHECK([whether $gltype is signed], [gl_cv_type_${gltype}_signed], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([$2[ int verify[2 * (($gltype) -1 < ($gltype) 0) - 1];]])], result=yes, result=no) eval gl_cv_type_${gltype}_signed=\$result ]) eval result=\$gl_cv_type_${gltype}_signed GLTYPE=`echo $gltype | tr 'abcdefghijklmnopqrstuvwxyz ' 'ABCDEFGHIJKLMNOPQRSTUVWXYZ_'` if test "$result" = yes; then AC_DEFINE_UNQUOTED([HAVE_SIGNED_${GLTYPE}], [1]) eval HAVE_SIGNED_${GLTYPE}=1 else eval HAVE_SIGNED_${GLTYPE}=0 fi done m4_foreach_w([gltype], [$1], [AC_SUBST([HAVE_SIGNED_]m4_translit(gltype,[abcdefghijklmnopqrstuvwxyz ],[ABCDEFGHIJKLMNOPQRSTUVWXYZ_]))]) ]) dnl gl_INTEGER_TYPE_SUFFIX(TYPES, INCLUDES) dnl Determine the suffix to use for integer constants of the given types. dnl Define t_SUFFIX for each such type. AC_DEFUN([gl_INTEGER_TYPE_SUFFIX], [ dnl Use a shell loop, to avoid bloating configure, and dnl - extra AH_TEMPLATE calls, so that autoheader knows what to put into dnl config.h.in, dnl - extra AC_SUBST calls, so that the right substitutions are made. m4_foreach_w([gltype], [$1], [AH_TEMPLATE(m4_translit(gltype,[abcdefghijklmnopqrstuvwxyz ],[ABCDEFGHIJKLMNOPQRSTUVWXYZ_])[_SUFFIX], [Define to l, ll, u, ul, ull, etc., as suitable for constants of type ']gltype['.])]) for gltype in $1 ; do AC_CACHE_CHECK([for $gltype integer literal suffix], [gl_cv_type_${gltype}_suffix], [eval gl_cv_type_${gltype}_suffix=no eval result=\$gl_cv_type_${gltype}_signed if test "$result" = yes; then glsufu= else glsufu=u fi for glsuf in "$glsufu" ${glsufu}l ${glsufu}ll ${glsufu}i64; do case $glsuf in '') gltype1='int';; l) gltype1='long int';; ll) gltype1='long long int';; i64) gltype1='__int64';; u) gltype1='unsigned int';; ul) gltype1='unsigned long int';; ull) gltype1='unsigned long long int';; ui64)gltype1='unsigned __int64';; esac AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([$2[ extern $gltype foo; extern $gltype1 foo;]])], [eval gl_cv_type_${gltype}_suffix=\$glsuf]) eval result=\$gl_cv_type_${gltype}_suffix test "$result" != no && break done]) GLTYPE=`echo $gltype | tr 'abcdefghijklmnopqrstuvwxyz ' 'ABCDEFGHIJKLMNOPQRSTUVWXYZ_'` eval result=\$gl_cv_type_${gltype}_suffix test "$result" = no && result= eval ${GLTYPE}_SUFFIX=\$result AC_DEFINE_UNQUOTED([${GLTYPE}_SUFFIX], [$result]) done m4_foreach_w([gltype], [$1], [AC_SUBST(m4_translit(gltype,[abcdefghijklmnopqrstuvwxyz ],[ABCDEFGHIJKLMNOPQRSTUVWXYZ_])[_SUFFIX])]) ]) dnl gl_STDINT_INCLUDES AC_DEFUN([gl_STDINT_INCLUDES], [[ /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif ]]) dnl gl_STDINT_TYPE_PROPERTIES dnl Compute HAVE_SIGNED_t, BITSIZEOF_t and t_SUFFIX, for all the types t dnl of interest to stdint.in.h. AC_DEFUN([gl_STDINT_TYPE_PROPERTIES], [ AC_REQUIRE([gl_MULTIARCH]) if test $APPLE_UNIVERSAL_BUILD = 0; then gl_STDINT_BITSIZEOF([ptrdiff_t size_t], [gl_STDINT_INCLUDES]) fi gl_STDINT_BITSIZEOF([sig_atomic_t wchar_t wint_t], [gl_STDINT_INCLUDES]) gl_CHECK_TYPES_SIGNED([sig_atomic_t wchar_t wint_t], [gl_STDINT_INCLUDES]) gl_cv_type_ptrdiff_t_signed=yes gl_cv_type_size_t_signed=no if test $APPLE_UNIVERSAL_BUILD = 0; then gl_INTEGER_TYPE_SUFFIX([ptrdiff_t size_t], [gl_STDINT_INCLUDES]) fi gl_INTEGER_TYPE_SUFFIX([sig_atomic_t wchar_t wint_t], [gl_STDINT_INCLUDES]) dnl If wint_t is smaller than 'int', it cannot satisfy the ISO C 99 dnl requirement that wint_t is "unchanged by default argument promotions". dnl In this case gnulib's and override wint_t. dnl Set the variable BITSIZEOF_WINT_T accordingly. if test $BITSIZEOF_WINT_T -lt 32; then BITSIZEOF_WINT_T=32 fi ]) dnl Autoconf >= 2.61 has AC_COMPUTE_INT built-in. dnl Remove this when we can assume autoconf >= 2.61. m4_ifdef([AC_COMPUTE_INT], [], [ AC_DEFUN([AC_COMPUTE_INT], [_AC_COMPUTE_INT([$2],[$1],[$3],[$4])]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/stddef_h.m40000644000175000017500000000321613004436755016176 00000000000000dnl A placeholder for , for platforms that have issues. # stddef_h.m4 serial 5 dnl Copyright (C) 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_STDDEF_H], [ AC_REQUIRE([gl_STDDEF_H_DEFAULTS]) AC_REQUIRE([gt_TYPE_WCHAR_T]) STDDEF_H= AC_CHECK_TYPE([max_align_t], [], [HAVE_MAX_ALIGN_T=0; STDDEF_H=stddef.h], [[#include ]]) if test $gt_cv_c_wchar_t = no; then HAVE_WCHAR_T=0 STDDEF_H=stddef.h fi AC_CACHE_CHECK([whether NULL can be used in arbitrary expressions], [gl_cv_decl_null_works], [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[#include int test[2 * (sizeof NULL == sizeof (void *)) -1]; ]])], [gl_cv_decl_null_works=yes], [gl_cv_decl_null_works=no])]) if test $gl_cv_decl_null_works = no; then REPLACE_NULL=1 STDDEF_H=stddef.h fi AC_SUBST([STDDEF_H]) AM_CONDITIONAL([GL_GENERATE_STDDEF_H], [test -n "$STDDEF_H"]) if test -n "$STDDEF_H"; then gl_NEXT_HEADERS([stddef.h]) fi ]) AC_DEFUN([gl_STDDEF_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_STDDEF_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) ]) AC_DEFUN([gl_STDDEF_H_DEFAULTS], [ dnl Assume proper GNU behavior unless another module says otherwise. REPLACE_NULL=0; AC_SUBST([REPLACE_NULL]) HAVE_MAX_ALIGN_T=1; AC_SUBST([HAVE_MAX_ALIGN_T]) HAVE_WCHAR_T=1; AC_SUBST([HAVE_WCHAR_T]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/stdbool.m40000644000175000017500000000672713004436755016076 00000000000000# Check for stdbool.h that conforms to C99. dnl Copyright (C) 2002-2006, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. #serial 7 # Prepare for substituting if it is not supported. AC_DEFUN([AM_STDBOOL_H], [ AC_REQUIRE([AC_CHECK_HEADER_STDBOOL]) # Define two additional variables used in the Makefile substitution. if test "$ac_cv_header_stdbool_h" = yes; then STDBOOL_H='' else STDBOOL_H='stdbool.h' fi AC_SUBST([STDBOOL_H]) AM_CONDITIONAL([GL_GENERATE_STDBOOL_H], [test -n "$STDBOOL_H"]) if test "$ac_cv_type__Bool" = yes; then HAVE__BOOL=1 else HAVE__BOOL=0 fi AC_SUBST([HAVE__BOOL]) ]) # AM_STDBOOL_H will be renamed to gl_STDBOOL_H in the future. AC_DEFUN([gl_STDBOOL_H], [AM_STDBOOL_H]) # This version of the macro is needed in autoconf <= 2.68. AC_DEFUN([AC_CHECK_HEADER_STDBOOL], [AC_CACHE_CHECK([for stdbool.h that conforms to C99], [ac_cv_header_stdbool_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[ #include #ifdef __cplusplus typedef bool Bool; #else typedef _Bool Bool; #ifndef bool "error: bool is not defined" #endif #ifndef false "error: false is not defined" #endif #if false "error: false is not 0" #endif #ifndef true "error: true is not defined" #endif #if true != 1 "error: true is not 1" #endif #endif #ifndef __bool_true_false_are_defined "error: __bool_true_false_are_defined is not defined" #endif struct s { Bool s: 1; Bool t; bool u: 1; bool v; } s; char a[true == 1 ? 1 : -1]; char b[false == 0 ? 1 : -1]; char c[__bool_true_false_are_defined == 1 ? 1 : -1]; char d[(bool) 0.5 == true ? 1 : -1]; /* See body of main program for 'e'. */ char f[(Bool) 0.0 == false ? 1 : -1]; char g[true]; char h[sizeof (Bool)]; char i[sizeof s.t]; enum { j = false, k = true, l = false * true, m = true * 256 }; /* The following fails for HP aC++/ANSI C B3910B A.05.55 [Dec 04 2003]. */ Bool n[m]; char o[sizeof n == m * sizeof n[0] ? 1 : -1]; char p[-1 - (Bool) 0 < 0 && -1 - (bool) 0 < 0 ? 1 : -1]; /* Catch a bug in an HP-UX C compiler. See http://gcc.gnu.org/ml/gcc-patches/2003-12/msg02303.html http://lists.gnu.org/archive/html/bug-coreutils/2005-11/msg00161.html */ Bool q = true; Bool *pq = &q; bool *qq = &q; ]], [[ bool e = &s; *pq |= q; *pq |= ! q; *qq |= q; *qq |= ! q; /* Refer to every declared value, to avoid compiler optimizations. */ return (!a + !b + !c + !d + !e + !f + !g + !h + !i + !!j + !k + !!l + !m + !n + !o + !p + !q + !pq + !qq); ]])], [ac_cv_header_stdbool_h=yes], [ac_cv_header_stdbool_h=no])]) AC_CHECK_TYPES([_Bool]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/stdalign.m40000644000175000017500000000437413004436755016231 00000000000000# Check for stdalign.h that conforms to C11. dnl Copyright 2011-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # Prepare for substituting if it is not supported. AC_DEFUN([gl_STDALIGN_H], [ AC_CACHE_CHECK([for working stdalign.h], [gl_cv_header_working_stdalign_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include #include /* Test that alignof yields a result consistent with offsetof. This catches GCC bug 52023 . */ #ifdef __cplusplus template struct alignof_helper { char a; t b; }; # define ao(type) offsetof (alignof_helper, b) #else # define ao(type) offsetof (struct { char a; type b; }, b) #endif char test_double[ao (double) % _Alignof (double) == 0 ? 1 : -1]; char test_long[ao (long int) % _Alignof (long int) == 0 ? 1 : -1]; char test_alignof[alignof (double) == _Alignof (double) ? 1 : -1]; /* Test _Alignas only on platforms where gnulib can help. */ #if \ ((defined __cplusplus && 201103 <= __cplusplus) \ || (defined __APPLE__ && defined __MACH__ \ ? 4 < __GNUC__ + (1 <= __GNUC_MINOR__) \ : __GNUC__) \ || __HP_cc || __HP_aCC || __IBMC__ || __IBMCPP__ \ || __ICC || 0x5110 <= __SUNPRO_C \ || 1300 <= _MSC_VER) struct alignas_test { char c; char alignas (8) alignas_8; }; char test_alignas[offsetof (struct alignas_test, alignas_8) == 8 ? 1 : -1]; #endif ]])], [gl_cv_header_working_stdalign_h=yes], [gl_cv_header_working_stdalign_h=no])]) if test $gl_cv_header_working_stdalign_h = yes; then STDALIGN_H='' else STDALIGN_H='stdalign.h' fi AC_SUBST([STDALIGN_H]) AM_CONDITIONAL([GL_GENERATE_STDALIGN_H], [test -n "$STDALIGN_H"]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/stat.m40000644000175000017500000000521413004436755015371 00000000000000# serial 11 # Copyright (C) 2009-2016 Free Software Foundation, Inc. # # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_STAT], [ AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_SYS_STAT_H_DEFAULTS]) AC_CHECK_FUNCS_ONCE([lstat]) dnl mingw is the only known platform where stat(".") and stat("./") differ AC_CACHE_CHECK([whether stat handles trailing slashes on directories], [gl_cv_func_stat_dir_slash], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[struct stat st; return stat (".", &st) != stat ("./", &st);]])], [gl_cv_func_stat_dir_slash=yes], [gl_cv_func_stat_dir_slash=no], [case $host_os in mingw*) gl_cv_func_stat_dir_slash="guessing no";; *) gl_cv_func_stat_dir_slash="guessing yes";; esac])]) dnl AIX 7.1, Solaris 9, mingw64 mistakenly succeed on stat("file/"). dnl (For mingw, this is due to a broken stat() override in libmingwex.a.) dnl FreeBSD 7.2 mistakenly succeeds on stat("link-to-file/"). AC_CACHE_CHECK([whether stat handles trailing slashes on files], [gl_cv_func_stat_file_slash], [touch conftest.tmp # Assume that if we have lstat, we can also check symlinks. if test $ac_cv_func_lstat = yes; then ln -s conftest.tmp conftest.lnk fi AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[int result = 0; struct stat st; if (!stat ("conftest.tmp/", &st)) result |= 1; #if HAVE_LSTAT if (!stat ("conftest.lnk/", &st)) result |= 2; #endif return result; ]])], [gl_cv_func_stat_file_slash=yes], [gl_cv_func_stat_file_slash=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_stat_file_slash="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_stat_file_slash="guessing no" ;; esac ]) rm -f conftest.tmp conftest.lnk]) case $gl_cv_func_stat_dir_slash in *no) REPLACE_STAT=1 AC_DEFINE([REPLACE_FUNC_STAT_DIR], [1], [Define to 1 if stat needs help when passed a directory name with a trailing slash]);; esac case $gl_cv_func_stat_file_slash in *no) REPLACE_STAT=1 AC_DEFINE([REPLACE_FUNC_STAT_FILE], [1], [Define to 1 if stat needs help when passed a file name with a trailing slash]);; esac ]) # Prerequisites of lib/stat.c. AC_DEFUN([gl_PREREQ_STAT], [:]) gnuastro-0.2.33-8a3b/bootstrapped/m4/ssize_t.m40000644000175000017500000000146313004436755016100 00000000000000# ssize_t.m4 serial 5 (gettext-0.18.2) dnl Copyright (C) 2001-2003, 2006, 2010-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl Test whether ssize_t is defined. AC_DEFUN([gt_TYPE_SSIZE_T], [ AC_CACHE_CHECK([for ssize_t], [gt_cv_ssize_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[int x = sizeof (ssize_t *) + sizeof (ssize_t); return !x;]])], [gt_cv_ssize_t=yes], [gt_cv_ssize_t=no])]) if test $gt_cv_ssize_t = no; then AC_DEFINE([ssize_t], [int], [Define as a signed type of the same size as size_t.]) fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/sleep.m40000644000175000017500000000403313004436755015524 00000000000000# sleep.m4 serial 7 dnl Copyright (C) 2007-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_SLEEP], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles dnl We expect to see the declaration of sleep() in a header file. dnl Older versions of mingw have a sleep() function that is an alias to dnl _sleep() in MSVCRT. It has a different signature than POSIX sleep(): dnl it takes the number of milliseconds as argument and returns void. dnl mingw does not declare this function. AC_CHECK_DECLS([sleep], , , [[#include ]]) AC_CHECK_FUNCS_ONCE([sleep]) if test $ac_cv_have_decl_sleep != yes; then HAVE_SLEEP=0 else dnl Cygwin 1.5.x has a bug where sleep can't exceed 49.7 days. AC_CACHE_CHECK([for working sleep], [gl_cv_func_sleep_works], [AC_RUN_IFELSE([AC_LANG_PROGRAM([[ #include #include #include static void handle_alarm (int sig) { if (sig != SIGALRM) _exit (2); } ]], [[ /* Failure to compile this test due to missing alarm is okay, since all such platforms (mingw) also lack sleep. */ unsigned int pentecost = 50 * 24 * 60 * 60; /* 50 days. */ unsigned int remaining; signal (SIGALRM, handle_alarm); alarm (1); remaining = sleep (pentecost); if (remaining > pentecost) return 3; if (remaining <= pentecost - 10) return 4; return 0; ]])], [gl_cv_func_sleep_works=yes], [gl_cv_func_sleep_works=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_sleep_works="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_sleep_works="guessing no" ;; esac ])]) case "$gl_cv_func_sleep_works" in *yes) ;; *) REPLACE_SLEEP=1 ;; esac fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/size_max.m40000644000175000017500000000577013004436755016244 00000000000000# size_max.m4 serial 10 dnl Copyright (C) 2003, 2005-2006, 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. AC_DEFUN([gl_SIZE_MAX], [ AC_CHECK_HEADERS([stdint.h]) dnl First test whether the system already has SIZE_MAX. AC_CACHE_CHECK([for SIZE_MAX], [gl_cv_size_max], [ gl_cv_size_max= AC_EGREP_CPP([Found it], [ #include #if HAVE_STDINT_H #include #endif #ifdef SIZE_MAX Found it #endif ], [gl_cv_size_max=yes]) if test -z "$gl_cv_size_max"; then dnl Define it ourselves. Here we assume that the type 'size_t' is not wider dnl than the type 'unsigned long'. Try hard to find a definition that can dnl be used in a preprocessor #if, i.e. doesn't contain a cast. AC_COMPUTE_INT([size_t_bits_minus_1], [sizeof (size_t) * CHAR_BIT - 1], [#include #include ], [size_t_bits_minus_1=]) AC_COMPUTE_INT([fits_in_uint], [sizeof (size_t) <= sizeof (unsigned int)], [#include ], [fits_in_uint=]) if test -n "$size_t_bits_minus_1" && test -n "$fits_in_uint"; then if test $fits_in_uint = 1; then dnl Even though SIZE_MAX fits in an unsigned int, it must be of type dnl 'unsigned long' if the type 'size_t' is the same as 'unsigned long'. AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include extern size_t foo; extern unsigned long foo; ]], [[]])], [fits_in_uint=0]) fi dnl We cannot use 'expr' to simplify this expression, because 'expr' dnl works only with 'long' integers in the host environment, while we dnl might be cross-compiling from a 32-bit platform to a 64-bit platform. if test $fits_in_uint = 1; then gl_cv_size_max="(((1U << $size_t_bits_minus_1) - 1) * 2 + 1)" else gl_cv_size_max="(((1UL << $size_t_bits_minus_1) - 1) * 2 + 1)" fi else dnl Shouldn't happen, but who knows... gl_cv_size_max='((size_t)~(size_t)0)' fi fi ]) if test "$gl_cv_size_max" != yes; then AC_DEFINE_UNQUOTED([SIZE_MAX], [$gl_cv_size_max], [Define as the maximum value of type 'size_t', if the system doesn't define it.]) fi dnl Don't redefine SIZE_MAX in config.h if config.h is re-included after dnl . Remember that the #undef in AH_VERBATIM gets replaced with dnl #define by AC_DEFINE_UNQUOTED. AH_VERBATIM([SIZE_MAX], [/* Define as the maximum value of type 'size_t', if the system doesn't define it. */ #ifndef SIZE_MAX # undef SIZE_MAX #endif]) ]) dnl Autoconf >= 2.61 has AC_COMPUTE_INT built-in. dnl Remove this when we can assume autoconf >= 2.61. m4_ifdef([AC_COMPUTE_INT], [], [ AC_DEFUN([AC_COMPUTE_INT], [_AC_COMPUTE_INT([$2],[$1],[$3],[$4])]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/setlocale.m40000644000175000017500000000154313004436755016372 00000000000000# setlocale.m4 serial 4 dnl Copyright (C) 2011-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_SETLOCALE], [ AC_REQUIRE([gl_LOCALE_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) case "$host_os" in dnl On native Windows systems, setlocale(category,NULL) does not look at dnl the environment variables LC_ALL, category, and LANG. mingw*) REPLACE_SETLOCALE=1 ;; dnl On Cygwin 1.5.x, setlocale always succeeds but setlocale(LC_CTYPE,NULL) dnl is then still "C". cygwin*) case `uname -r` in 1.5.*) REPLACE_SETLOCALE=1 ;; esac ;; esac ]) # Prerequisites of lib/setlocale.c. AC_DEFUN([gl_PREREQ_SETLOCALE], [ : ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/setenv.m40000644000175000017500000001101213004436755015713 00000000000000# setenv.m4 serial 26 dnl Copyright (C) 2001-2004, 2006-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_SETENV], [ AC_REQUIRE([gl_FUNC_SETENV_SEPARATE]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles if test $ac_cv_func_setenv = no; then HAVE_SETENV=0 else AC_CACHE_CHECK([whether setenv validates arguments], [gl_cv_func_setenv_works], [AC_RUN_IFELSE([AC_LANG_PROGRAM([[ #include #include #include ]], [[ int result = 0; { if (setenv ("", "", 0) != -1) result |= 1; else if (errno != EINVAL) result |= 2; } { if (setenv ("a", "=", 1) != 0) result |= 4; else if (strcmp (getenv ("a"), "=") != 0) result |= 8; } return result; ]])], [gl_cv_func_setenv_works=yes], [gl_cv_func_setenv_works=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_setenv_works="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_setenv_works="guessing no" ;; esac ])]) case "$gl_cv_func_setenv_works" in *yes) ;; *) REPLACE_SETENV=1 ;; esac fi ]) # Like gl_FUNC_SETENV, except prepare for separate compilation # (no REPLACE_SETENV, no AC_LIBOBJ). AC_DEFUN([gl_FUNC_SETENV_SEPARATE], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) AC_CHECK_DECLS_ONCE([setenv]) if test $ac_cv_have_decl_setenv = no; then HAVE_DECL_SETENV=0 fi AC_CHECK_FUNCS_ONCE([setenv]) gl_PREREQ_SETENV ]) AC_DEFUN([gl_FUNC_UNSETENV], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CHECK_DECLS_ONCE([unsetenv]) if test $ac_cv_have_decl_unsetenv = no; then HAVE_DECL_UNSETENV=0 fi AC_CHECK_FUNCS([unsetenv]) if test $ac_cv_func_unsetenv = no; then HAVE_UNSETENV=0 else HAVE_UNSETENV=1 dnl Some BSDs return void, failing to do error checking. AC_CACHE_CHECK([for unsetenv() return type], [gt_cv_func_unsetenv_ret], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[ #undef _BSD #define _BSD 1 /* unhide unsetenv declaration in OSF/1 5.1 */ #include extern #ifdef __cplusplus "C" #endif int unsetenv (const char *name); ]], [[]])], [gt_cv_func_unsetenv_ret='int'], [gt_cv_func_unsetenv_ret='void'])]) if test $gt_cv_func_unsetenv_ret = 'void'; then AC_DEFINE([VOID_UNSETENV], [1], [Define to 1 if unsetenv returns void instead of int.]) REPLACE_UNSETENV=1 fi dnl Solaris 10 unsetenv does not remove all copies of a name. dnl Haiku alpha 2 unsetenv gets confused by assignment to environ. dnl OpenBSD 4.7 unsetenv("") does not fail. AC_CACHE_CHECK([whether unsetenv obeys POSIX], [gl_cv_func_unsetenv_works], [AC_RUN_IFELSE([AC_LANG_PROGRAM([[ #include #include extern char **environ; ]], [[ char entry1[] = "a=1"; char entry2[] = "b=2"; char *env[] = { entry1, entry2, NULL }; if (putenv ((char *) "a=1")) return 1; if (putenv (entry2)) return 2; entry2[0] = 'a'; unsetenv ("a"); if (getenv ("a")) return 3; if (!unsetenv ("") || errno != EINVAL) return 4; entry2[0] = 'b'; environ = env; if (!getenv ("a")) return 5; entry2[0] = 'a'; unsetenv ("a"); if (getenv ("a")) return 6; ]])], [gl_cv_func_unsetenv_works=yes], [gl_cv_func_unsetenv_works=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_unsetenv_works="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_unsetenv_works="guessing no" ;; esac ])]) case "$gl_cv_func_unsetenv_works" in *yes) ;; *) REPLACE_UNSETENV=1 ;; esac fi ]) # Prerequisites of lib/setenv.c. AC_DEFUN([gl_PREREQ_SETENV], [ AC_REQUIRE([AC_FUNC_ALLOCA]) AC_REQUIRE([gl_ENVIRON]) AC_CHECK_HEADERS_ONCE([unistd.h]) AC_CHECK_HEADERS([search.h]) AC_CHECK_FUNCS([tsearch]) ]) # Prerequisites of lib/unsetenv.c. AC_DEFUN([gl_PREREQ_UNSETENV], [ AC_REQUIRE([gl_ENVIRON]) AC_CHECK_HEADERS_ONCE([unistd.h]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/regex.m40000644000175000017500000002726713004436755015544 00000000000000# serial 66 # Copyright (C) 1996-2001, 2003-2016 Free Software Foundation, Inc. # # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. dnl Initially derived from code in GNU grep. dnl Mostly written by Jim Meyering. AC_PREREQ([2.50]) AC_DEFUN([gl_REGEX], [ AC_ARG_WITH([included-regex], [AS_HELP_STRING([--without-included-regex], [don't compile regex; this is the default on systems with recent-enough versions of the GNU C Library (use with caution on other systems).])]) case $with_included_regex in #( yes|no) ac_use_included_regex=$with_included_regex ;; '') # If the system regex support is good enough that it passes the # following run test, then default to *not* using the included regex.c. # If cross compiling, assume the test would fail and use the included # regex.c. AC_CHECK_DECLS_ONCE([alarm]) AC_CHECK_HEADERS_ONCE([malloc.h]) AC_CACHE_CHECK([for working re_compile_pattern], [gl_cv_func_re_compile_pattern_working], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include #include #include #if defined M_CHECK_ACTION || HAVE_DECL_ALARM # include # include #endif #if HAVE_MALLOC_H # include #endif #ifdef M_CHECK_ACTION /* Exit with distinguishable exit code. */ static void sigabrt_no_core (int sig) { raise (SIGTERM); } #endif ]], [[int result = 0; static struct re_pattern_buffer regex; unsigned char folded_chars[UCHAR_MAX + 1]; int i; const char *s; struct re_registers regs; /* Some builds of glibc go into an infinite loop on this test. Use alarm to force death, and mallopt to avoid malloc recursion in diagnosing the corrupted heap. */ #if HAVE_DECL_ALARM signal (SIGALRM, SIG_DFL); alarm (2); #endif #ifdef M_CHECK_ACTION signal (SIGABRT, sigabrt_no_core); mallopt (M_CHECK_ACTION, 2); #endif if (setlocale (LC_ALL, "en_US.UTF-8")) { { /* http://sourceware.org/ml/libc-hacker/2006-09/msg00008.html This test needs valgrind to catch the bug on Debian GNU/Linux 3.1 x86, but it might catch the bug better on other platforms and it shouldn't hurt to try the test here. */ static char const pat[] = "insert into"; static char const data[] = "\xFF\0\x12\xA2\xAA\xC4\xB1,K\x12\xC4\xB1*\xACK"; re_set_syntax (RE_SYNTAX_GREP | RE_HAT_LISTS_NOT_NEWLINE | RE_ICASE); memset (®ex, 0, sizeof regex); s = re_compile_pattern (pat, sizeof pat - 1, ®ex); if (s) result |= 1; else if (re_search (®ex, data, sizeof data - 1, 0, sizeof data - 1, ®s) != -1) result |= 1; regfree (®ex); } { /* This test is from glibc bug 15078. The test case is from Andreas Schwab in . */ static char const pat[] = "[^x]x"; static char const data[] = /* */ "\xe1\x80\x80" "\xe1\x80\xbb" "\xe1\x80\xbd" "\xe1\x80\x94" "\xe1\x80\xba" "\xe1\x80\xaf" "\xe1\x80\x95" "\xe1\x80\xba" "x"; re_set_syntax (0); memset (®ex, 0, sizeof regex); s = re_compile_pattern (pat, sizeof pat - 1, ®ex); if (s) result |= 1; else { i = re_search (®ex, data, sizeof data - 1, 0, sizeof data - 1, 0); if (i != 0 && i != 21) result |= 1; } regfree (®ex); } if (! setlocale (LC_ALL, "C")) return 1; } /* This test is from glibc bug 3957, reported by Andrew Mackey. */ re_set_syntax (RE_SYNTAX_EGREP | RE_HAT_LISTS_NOT_NEWLINE); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("a[^x]b", 6, ®ex); if (s) result |= 2; /* This should fail, but succeeds for glibc-2.5. */ else if (re_search (®ex, "a\nb", 3, 0, 3, ®s) != -1) result |= 2; /* This regular expression is from Spencer ere test number 75 in grep-2.3. */ re_set_syntax (RE_SYNTAX_POSIX_EGREP); memset (®ex, 0, sizeof regex); for (i = 0; i <= UCHAR_MAX; i++) folded_chars[i] = i; regex.translate = folded_chars; s = re_compile_pattern ("a[[:@:>@:]]b\n", 11, ®ex); /* This should fail with _Invalid character class name_ error. */ if (!s) result |= 4; /* Ensure that [b-a] is diagnosed as invalid, when using RE_NO_EMPTY_RANGES. */ re_set_syntax (RE_SYNTAX_POSIX_EGREP | RE_NO_EMPTY_RANGES); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("a[b-a]", 6, ®ex); if (s == 0) result |= 8; /* This should succeed, but does not for glibc-2.1.3. */ memset (®ex, 0, sizeof regex); s = re_compile_pattern ("{1", 2, ®ex); if (s) result |= 8; /* The following example is derived from a problem report against gawk from Jorge Stolfi . */ memset (®ex, 0, sizeof regex); s = re_compile_pattern ("[an\371]*n", 7, ®ex); if (s) result |= 8; /* This should match, but does not for glibc-2.2.1. */ else if (re_match (®ex, "an", 2, 0, ®s) != 2) result |= 8; memset (®ex, 0, sizeof regex); s = re_compile_pattern ("x", 1, ®ex); if (s) result |= 8; /* glibc-2.2.93 does not work with a negative RANGE argument. */ else if (re_search (®ex, "wxy", 3, 2, -2, ®s) != 1) result |= 8; /* The version of regex.c in older versions of gnulib ignored RE_ICASE. Detect that problem too. */ re_set_syntax (RE_SYNTAX_EMACS | RE_ICASE); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("x", 1, ®ex); if (s) result |= 16; else if (re_search (®ex, "WXY", 3, 0, 3, ®s) < 0) result |= 16; /* Catch a bug reported by Vin Shelton in http://lists.gnu.org/archive/html/bug-coreutils/2007-06/msg00089.html */ re_set_syntax (RE_SYNTAX_POSIX_BASIC & ~RE_CONTEXT_INVALID_DUP & ~RE_NO_EMPTY_RANGES); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("[[:alnum:]_-]\\\\+$", 16, ®ex); if (s) result |= 32; /* REG_STARTEND was added to glibc on 2004-01-15. Reject older versions. */ if (! REG_STARTEND) result |= 64; #if 0 /* It would be nice to reject hosts whose regoff_t values are too narrow (including glibc on hosts with 64-bit ptrdiff_t and 32-bit int), but we should wait until glibc implements this feature. Otherwise, support for equivalence classes and multibyte collation symbols would always be broken except when compiling --without-included-regex. */ if (sizeof (regoff_t) < sizeof (ptrdiff_t) || sizeof (regoff_t) < sizeof (ssize_t)) result |= 64; #endif return result; ]])], [gl_cv_func_re_compile_pattern_working=yes], [gl_cv_func_re_compile_pattern_working=no], dnl When crosscompiling, assume it is not working. [gl_cv_func_re_compile_pattern_working=no])]) case $gl_cv_func_re_compile_pattern_working in #( yes) ac_use_included_regex=no;; #( no) ac_use_included_regex=yes;; esac ;; *) AC_MSG_ERROR([Invalid value for --with-included-regex: $with_included_regex]) ;; esac if test $ac_use_included_regex = yes; then AC_DEFINE([_REGEX_INCLUDE_LIMITS_H], [1], [Define if you want to include , so that it consistently overrides 's RE_DUP_MAX.]) AC_DEFINE([_REGEX_LARGE_OFFSETS], [1], [Define if you want regoff_t to be at least as wide POSIX requires.]) AC_DEFINE([re_syntax_options], [rpl_re_syntax_options], [Define to rpl_re_syntax_options if the replacement should be used.]) AC_DEFINE([re_set_syntax], [rpl_re_set_syntax], [Define to rpl_re_set_syntax if the replacement should be used.]) AC_DEFINE([re_compile_pattern], [rpl_re_compile_pattern], [Define to rpl_re_compile_pattern if the replacement should be used.]) AC_DEFINE([re_compile_fastmap], [rpl_re_compile_fastmap], [Define to rpl_re_compile_fastmap if the replacement should be used.]) AC_DEFINE([re_search], [rpl_re_search], [Define to rpl_re_search if the replacement should be used.]) AC_DEFINE([re_search_2], [rpl_re_search_2], [Define to rpl_re_search_2 if the replacement should be used.]) AC_DEFINE([re_match], [rpl_re_match], [Define to rpl_re_match if the replacement should be used.]) AC_DEFINE([re_match_2], [rpl_re_match_2], [Define to rpl_re_match_2 if the replacement should be used.]) AC_DEFINE([re_set_registers], [rpl_re_set_registers], [Define to rpl_re_set_registers if the replacement should be used.]) AC_DEFINE([re_comp], [rpl_re_comp], [Define to rpl_re_comp if the replacement should be used.]) AC_DEFINE([re_exec], [rpl_re_exec], [Define to rpl_re_exec if the replacement should be used.]) AC_DEFINE([regcomp], [rpl_regcomp], [Define to rpl_regcomp if the replacement should be used.]) AC_DEFINE([regexec], [rpl_regexec], [Define to rpl_regexec if the replacement should be used.]) AC_DEFINE([regerror], [rpl_regerror], [Define to rpl_regerror if the replacement should be used.]) AC_DEFINE([regfree], [rpl_regfree], [Define to rpl_regfree if the replacement should be used.]) fi ]) # Prerequisites of lib/regex.c and lib/regex_internal.c. AC_DEFUN([gl_PREREQ_REGEX], [ AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([AC_C_INLINE]) AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([AC_TYPE_MBSTATE_T]) AC_REQUIRE([gl_EEMALLOC]) AC_REQUIRE([gl_GLIBC21]) AC_CHECK_HEADERS([libintl.h]) AC_CHECK_FUNCS_ONCE([isblank iswctype]) AC_CHECK_DECLS([isblank], [], [], [[#include ]]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/rawmemchr.m40000644000175000017500000000117213004436755016402 00000000000000# rawmemchr.m4 serial 2 dnl Copyright (C) 2003, 2007-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_RAWMEMCHR], [ dnl Persuade glibc to declare rawmemchr(). AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) AC_CHECK_FUNCS([rawmemchr]) if test $ac_cv_func_rawmemchr = no; then HAVE_RAWMEMCHR=0 fi ]) # Prerequisites of lib/strchrnul.c. AC_DEFUN([gl_PREREQ_RAWMEMCHR], [:]) gnuastro-0.2.33-8a3b/bootstrapped/m4/putenv.m40000644000175000017500000000317513004436755015743 00000000000000# putenv.m4 serial 20 dnl Copyright (C) 2002-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Jim Meyering. dnl dnl Check whether putenv ("FOO") removes FOO from the environment. dnl The putenv in libc on at least SunOS 4.1.4 does *not* do that. AC_DEFUN([gl_FUNC_PUTENV], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([for putenv compatible with GNU and SVID], [gl_cv_func_svid_putenv], [AC_RUN_IFELSE([AC_LANG_PROGRAM([AC_INCLUDES_DEFAULT],[[ /* Put it in env. */ if (putenv ("CONFTEST_putenv=val")) return 1; /* Try to remove it. */ if (putenv ("CONFTEST_putenv")) return 2; /* Make sure it was deleted. */ if (getenv ("CONFTEST_putenv") != 0) return 3; return 0; ]])], gl_cv_func_svid_putenv=yes, gl_cv_func_svid_putenv=no, dnl When crosscompiling, assume putenv is broken. [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_svid_putenv="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_svid_putenv="guessing no" ;; esac ]) ]) case "$gl_cv_func_svid_putenv" in *yes) ;; *) REPLACE_PUTENV=1 ;; esac ]) # Prerequisites of lib/putenv.c. AC_DEFUN([gl_PREREQ_PUTENV], [ AC_CHECK_DECLS([_putenv]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/printf.m40000644000175000017500000016517013004436755015730 00000000000000# printf.m4 serial 52 dnl Copyright (C) 2003, 2007-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Test whether the *printf family of functions supports the 'j', 'z', 't', dnl 'L' size specifiers. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_printf_sizes_c99. AC_DEFUN([gl_PRINTF_SIZES_C99], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gl_AC_HEADER_STDINT_H]) AC_REQUIRE([gl_AC_HEADER_INTTYPES_H]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports size specifiers as in C99], [gl_cv_func_printf_sizes_c99], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include #include #if HAVE_STDINT_H_WITH_UINTMAX # include #endif #if HAVE_INTTYPES_H_WITH_UINTMAX # include #endif static char buf[100]; int main () { int result = 0; #if HAVE_STDINT_H_WITH_UINTMAX || HAVE_INTTYPES_H_WITH_UINTMAX buf[0] = '\0'; if (sprintf (buf, "%ju %d", (uintmax_t) 12345671, 33, 44, 55) < 0 || strcmp (buf, "12345671 33") != 0) result |= 1; #else result |= 1; #endif buf[0] = '\0'; if (sprintf (buf, "%zu %d", (size_t) 12345672, 33, 44, 55) < 0 || strcmp (buf, "12345672 33") != 0) result |= 2; buf[0] = '\0'; if (sprintf (buf, "%tu %d", (ptrdiff_t) 12345673, 33, 44, 55) < 0 || strcmp (buf, "12345673 33") != 0) result |= 4; buf[0] = '\0'; if (sprintf (buf, "%Lg %d", (long double) 1.5, 33, 44, 55) < 0 || strcmp (buf, "1.5 33") != 0) result |= 8; return result; }]])], [gl_cv_func_printf_sizes_c99=yes], [gl_cv_func_printf_sizes_c99=no], [ changequote(,)dnl case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_printf_sizes_c99="guessing yes";; # Guess yes on FreeBSD >= 5. freebsd[1-4].*) gl_cv_func_printf_sizes_c99="guessing no";; freebsd* | kfreebsd*) gl_cv_func_printf_sizes_c99="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_printf_sizes_c99="guessing no";; darwin*) gl_cv_func_printf_sizes_c99="guessing yes";; # Guess yes on OpenBSD >= 3.9. openbsd[1-2].* | openbsd3.[0-8] | openbsd3.[0-8].*) gl_cv_func_printf_sizes_c99="guessing no";; openbsd*) gl_cv_func_printf_sizes_c99="guessing yes";; # Guess yes on Solaris >= 2.10. solaris2.[1-9][0-9]*) gl_cv_func_printf_sizes_c99="guessing yes";; solaris*) gl_cv_func_printf_sizes_c99="guessing no";; # Guess yes on NetBSD >= 3. netbsd[1-2]* | netbsdelf[1-2]* | netbsdaout[1-2]* | netbsdcoff[1-2]*) gl_cv_func_printf_sizes_c99="guessing no";; netbsd*) gl_cv_func_printf_sizes_c99="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_printf_sizes_c99="guessing no";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions supports 'long double' dnl arguments together with the 'L' size specifier. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_printf_long_double. AC_DEFUN([gl_PRINTF_LONG_DOUBLE], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports 'long double' arguments], [gl_cv_func_printf_long_double], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static char buf[10000]; int main () { int result = 0; buf[0] = '\0'; if (sprintf (buf, "%Lf %d", 1.75L, 33, 44, 55) < 0 || strcmp (buf, "1.750000 33") != 0) result |= 1; buf[0] = '\0'; if (sprintf (buf, "%Le %d", 1.75L, 33, 44, 55) < 0 || strcmp (buf, "1.750000e+00 33") != 0) result |= 2; buf[0] = '\0'; if (sprintf (buf, "%Lg %d", 1.75L, 33, 44, 55) < 0 || strcmp (buf, "1.75 33") != 0) result |= 4; return result; }]])], [gl_cv_func_printf_long_double=yes], [gl_cv_func_printf_long_double=no], [ changequote(,)dnl case "$host_os" in beos*) gl_cv_func_printf_long_double="guessing no";; mingw* | pw*) gl_cv_func_printf_long_double="guessing no";; *) gl_cv_func_printf_long_double="guessing yes";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions supports infinite and NaN dnl 'double' arguments and negative zero arguments in the %f, %e, %g dnl directives. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_printf_infinite. AC_DEFUN([gl_PRINTF_INFINITE], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports infinite 'double' arguments], [gl_cv_func_printf_infinite], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static int strisnan (const char *string, size_t start_index, size_t end_index) { if (start_index < end_index) { if (string[start_index] == '-') start_index++; if (start_index + 3 <= end_index && memcmp (string + start_index, "nan", 3) == 0) { start_index += 3; if (start_index == end_index || (string[start_index] == '(' && string[end_index - 1] == ')')) return 1; } } return 0; } static int have_minus_zero () { static double plus_zero = 0.0; double minus_zero = - plus_zero; return memcmp (&plus_zero, &minus_zero, sizeof (double)) != 0; } static char buf[10000]; static double zero = 0.0; int main () { int result = 0; if (sprintf (buf, "%f", 1.0 / zero) < 0 || (strcmp (buf, "inf") != 0 && strcmp (buf, "infinity") != 0)) result |= 1; if (sprintf (buf, "%f", -1.0 / zero) < 0 || (strcmp (buf, "-inf") != 0 && strcmp (buf, "-infinity") != 0)) result |= 1; if (sprintf (buf, "%f", zero / zero) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 2; if (sprintf (buf, "%e", 1.0 / zero) < 0 || (strcmp (buf, "inf") != 0 && strcmp (buf, "infinity") != 0)) result |= 4; if (sprintf (buf, "%e", -1.0 / zero) < 0 || (strcmp (buf, "-inf") != 0 && strcmp (buf, "-infinity") != 0)) result |= 4; if (sprintf (buf, "%e", zero / zero) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 8; if (sprintf (buf, "%g", 1.0 / zero) < 0 || (strcmp (buf, "inf") != 0 && strcmp (buf, "infinity") != 0)) result |= 16; if (sprintf (buf, "%g", -1.0 / zero) < 0 || (strcmp (buf, "-inf") != 0 && strcmp (buf, "-infinity") != 0)) result |= 16; if (sprintf (buf, "%g", zero / zero) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 32; /* This test fails on HP-UX 10.20. */ if (have_minus_zero ()) if (sprintf (buf, "%g", - zero) < 0 || strcmp (buf, "-0") != 0) result |= 64; return result; }]])], [gl_cv_func_printf_infinite=yes], [gl_cv_func_printf_infinite=no], [ changequote(,)dnl case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_printf_infinite="guessing yes";; # Guess yes on FreeBSD >= 6. freebsd[1-5].*) gl_cv_func_printf_infinite="guessing no";; freebsd* | kfreebsd*) gl_cv_func_printf_infinite="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_printf_infinite="guessing no";; darwin*) gl_cv_func_printf_infinite="guessing yes";; # Guess yes on HP-UX >= 11. hpux[7-9]* | hpux10*) gl_cv_func_printf_infinite="guessing no";; hpux*) gl_cv_func_printf_infinite="guessing yes";; # Guess yes on NetBSD >= 3. netbsd[1-2]* | netbsdelf[1-2]* | netbsdaout[1-2]* | netbsdcoff[1-2]*) gl_cv_func_printf_infinite="guessing no";; netbsd*) gl_cv_func_printf_infinite="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_printf_infinite="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_printf_infinite="guessing no";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions supports infinite and NaN dnl 'long double' arguments in the %f, %e, %g directives. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_printf_infinite_long_double. AC_DEFUN([gl_PRINTF_INFINITE_LONG_DOUBLE], [ AC_REQUIRE([gl_PRINTF_LONG_DOUBLE]) AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gl_BIGENDIAN]) AC_REQUIRE([gl_LONG_DOUBLE_VS_DOUBLE]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles dnl The user can set or unset the variable gl_printf_safe to indicate dnl that he wishes a safe handling of non-IEEE-754 'long double' values. if test -n "$gl_printf_safe"; then AC_DEFINE([CHECK_PRINTF_SAFE], [1], [Define if you wish *printf() functions that have a safe handling of non-IEEE-754 'long double' values.]) fi case "$gl_cv_func_printf_long_double" in *yes) AC_CACHE_CHECK([whether printf supports infinite 'long double' arguments], [gl_cv_func_printf_infinite_long_double], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ ]GL_NOCRASH[ #include #include #include static int strisnan (const char *string, size_t start_index, size_t end_index) { if (start_index < end_index) { if (string[start_index] == '-') start_index++; if (start_index + 3 <= end_index && memcmp (string + start_index, "nan", 3) == 0) { start_index += 3; if (start_index == end_index || (string[start_index] == '(' && string[end_index - 1] == ')')) return 1; } } return 0; } static char buf[10000]; static long double zeroL = 0.0L; int main () { int result = 0; nocrash_init(); if (sprintf (buf, "%Lf", 1.0L / zeroL) < 0 || (strcmp (buf, "inf") != 0 && strcmp (buf, "infinity") != 0)) result |= 1; if (sprintf (buf, "%Lf", -1.0L / zeroL) < 0 || (strcmp (buf, "-inf") != 0 && strcmp (buf, "-infinity") != 0)) result |= 1; if (sprintf (buf, "%Lf", zeroL / zeroL) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 1; if (sprintf (buf, "%Le", 1.0L / zeroL) < 0 || (strcmp (buf, "inf") != 0 && strcmp (buf, "infinity") != 0)) result |= 1; if (sprintf (buf, "%Le", -1.0L / zeroL) < 0 || (strcmp (buf, "-inf") != 0 && strcmp (buf, "-infinity") != 0)) result |= 1; if (sprintf (buf, "%Le", zeroL / zeroL) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 1; if (sprintf (buf, "%Lg", 1.0L / zeroL) < 0 || (strcmp (buf, "inf") != 0 && strcmp (buf, "infinity") != 0)) result |= 1; if (sprintf (buf, "%Lg", -1.0L / zeroL) < 0 || (strcmp (buf, "-inf") != 0 && strcmp (buf, "-infinity") != 0)) result |= 1; if (sprintf (buf, "%Lg", zeroL / zeroL) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 1; #if CHECK_PRINTF_SAFE && ((defined __ia64 && LDBL_MANT_DIG == 64) || (defined __x86_64__ || defined __amd64__) || (defined __i386 || defined __i386__ || defined _I386 || defined _M_IX86 || defined _X86_)) && !HAVE_SAME_LONG_DOUBLE_AS_DOUBLE /* Representation of an 80-bit 'long double' as an initializer for a sequence of 'unsigned int' words. */ # ifdef WORDS_BIGENDIAN # define LDBL80_WORDS(exponent,manthi,mantlo) \ { ((unsigned int) (exponent) << 16) | ((unsigned int) (manthi) >> 16), \ ((unsigned int) (manthi) << 16) | ((unsigned int) (mantlo) >> 16), \ (unsigned int) (mantlo) << 16 \ } # else # define LDBL80_WORDS(exponent,manthi,mantlo) \ { mantlo, manthi, exponent } # endif { /* Quiet NaN. */ static union { unsigned int word[4]; long double value; } x = { LDBL80_WORDS (0xFFFF, 0xC3333333, 0x00000000) }; if (sprintf (buf, "%Lf", x.value) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 2; if (sprintf (buf, "%Le", x.value) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 2; if (sprintf (buf, "%Lg", x.value) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 2; } { /* Signalling NaN. */ static union { unsigned int word[4]; long double value; } x = { LDBL80_WORDS (0xFFFF, 0x83333333, 0x00000000) }; if (sprintf (buf, "%Lf", x.value) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 2; if (sprintf (buf, "%Le", x.value) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 2; if (sprintf (buf, "%Lg", x.value) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 2; } { /* Pseudo-NaN. */ static union { unsigned int word[4]; long double value; } x = { LDBL80_WORDS (0xFFFF, 0x40000001, 0x00000000) }; if (sprintf (buf, "%Lf", x.value) <= 0) result |= 4; if (sprintf (buf, "%Le", x.value) <= 0) result |= 4; if (sprintf (buf, "%Lg", x.value) <= 0) result |= 4; } { /* Pseudo-Infinity. */ static union { unsigned int word[4]; long double value; } x = { LDBL80_WORDS (0xFFFF, 0x00000000, 0x00000000) }; if (sprintf (buf, "%Lf", x.value) <= 0) result |= 8; if (sprintf (buf, "%Le", x.value) <= 0) result |= 8; if (sprintf (buf, "%Lg", x.value) <= 0) result |= 8; } { /* Pseudo-Zero. */ static union { unsigned int word[4]; long double value; } x = { LDBL80_WORDS (0x4004, 0x00000000, 0x00000000) }; if (sprintf (buf, "%Lf", x.value) <= 0) result |= 16; if (sprintf (buf, "%Le", x.value) <= 0) result |= 16; if (sprintf (buf, "%Lg", x.value) <= 0) result |= 16; } { /* Unnormalized number. */ static union { unsigned int word[4]; long double value; } x = { LDBL80_WORDS (0x4000, 0x63333333, 0x00000000) }; if (sprintf (buf, "%Lf", x.value) <= 0) result |= 32; if (sprintf (buf, "%Le", x.value) <= 0) result |= 32; if (sprintf (buf, "%Lg", x.value) <= 0) result |= 32; } { /* Pseudo-Denormal. */ static union { unsigned int word[4]; long double value; } x = { LDBL80_WORDS (0x0000, 0x83333333, 0x00000000) }; if (sprintf (buf, "%Lf", x.value) <= 0) result |= 64; if (sprintf (buf, "%Le", x.value) <= 0) result |= 64; if (sprintf (buf, "%Lg", x.value) <= 0) result |= 64; } #endif return result; }]])], [gl_cv_func_printf_infinite_long_double=yes], [gl_cv_func_printf_infinite_long_double=no], [ changequote(,)dnl case "$host_cpu" in # Guess no on ia64, x86_64, i386. ia64 | x86_64 | i*86) gl_cv_func_printf_infinite_long_double="guessing no";; *) case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_printf_infinite_long_double="guessing yes";; # Guess yes on FreeBSD >= 6. freebsd[1-5].*) gl_cv_func_printf_infinite_long_double="guessing no";; freebsd* | kfreebsd*) gl_cv_func_printf_infinite_long_double="guessing yes";; # Guess yes on HP-UX >= 11. hpux[7-9]* | hpux10*) gl_cv_func_printf_infinite_long_double="guessing no";; hpux*) gl_cv_func_printf_infinite_long_double="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_printf_infinite_long_double="guessing no";; esac ;; esac changequote([,])dnl ]) ]) ;; *) gl_cv_func_printf_infinite_long_double="irrelevant" ;; esac ]) dnl Test whether the *printf family of functions supports the 'a' and 'A' dnl conversion specifier for hexadecimal output of floating-point numbers. dnl (ISO C99, POSIX:2001) dnl Result is gl_cv_func_printf_directive_a. AC_DEFUN([gl_PRINTF_DIRECTIVE_A], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports the 'a' and 'A' directives], [gl_cv_func_printf_directive_a], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static char buf[100]; static double zero = 0.0; int main () { int result = 0; if (sprintf (buf, "%a %d", 3.1416015625, 33, 44, 55) < 0 || (strcmp (buf, "0x1.922p+1 33") != 0 && strcmp (buf, "0x3.244p+0 33") != 0 && strcmp (buf, "0x6.488p-1 33") != 0 && strcmp (buf, "0xc.91p-2 33") != 0)) result |= 1; if (sprintf (buf, "%A %d", -3.1416015625, 33, 44, 55) < 0 || (strcmp (buf, "-0X1.922P+1 33") != 0 && strcmp (buf, "-0X3.244P+0 33") != 0 && strcmp (buf, "-0X6.488P-1 33") != 0 && strcmp (buf, "-0XC.91P-2 33") != 0)) result |= 2; /* This catches a FreeBSD 6.1 bug: it doesn't round. */ if (sprintf (buf, "%.2a %d", 1.51, 33, 44, 55) < 0 || (strcmp (buf, "0x1.83p+0 33") != 0 && strcmp (buf, "0x3.05p-1 33") != 0 && strcmp (buf, "0x6.0ap-2 33") != 0 && strcmp (buf, "0xc.14p-3 33") != 0)) result |= 4; /* This catches a FreeBSD 6.1 bug. See */ if (sprintf (buf, "%010a %d", 1.0 / zero, 33, 44, 55) < 0 || buf[0] == '0') result |= 8; /* This catches a Mac OS X 10.3.9 (Darwin 7.9) bug. */ if (sprintf (buf, "%.1a", 1.999) < 0 || (strcmp (buf, "0x1.0p+1") != 0 && strcmp (buf, "0x2.0p+0") != 0 && strcmp (buf, "0x4.0p-1") != 0 && strcmp (buf, "0x8.0p-2") != 0)) result |= 16; /* This catches the same Mac OS X 10.3.9 (Darwin 7.9) bug and also a glibc 2.4 bug . */ if (sprintf (buf, "%.1La", 1.999L) < 0 || (strcmp (buf, "0x1.0p+1") != 0 && strcmp (buf, "0x2.0p+0") != 0 && strcmp (buf, "0x4.0p-1") != 0 && strcmp (buf, "0x8.0p-2") != 0)) result |= 32; return result; }]])], [gl_cv_func_printf_directive_a=yes], [gl_cv_func_printf_directive_a=no], [ case "$host_os" in # Guess yes on glibc >= 2.5 systems. *-gnu*) AC_EGREP_CPP([BZ2908], [ #include #ifdef __GNU_LIBRARY__ #if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 5) || (__GLIBC__ > 2)) && !defined __UCLIBC__ BZ2908 #endif #endif ], [gl_cv_func_printf_directive_a="guessing yes"], [gl_cv_func_printf_directive_a="guessing no"]) ;; # If we don't know, assume the worst. *) gl_cv_func_printf_directive_a="guessing no";; esac ]) ]) ]) dnl Test whether the *printf family of functions supports the %F format dnl directive. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_printf_directive_f. AC_DEFUN([gl_PRINTF_DIRECTIVE_F], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports the 'F' directive], [gl_cv_func_printf_directive_f], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static char buf[100]; static double zero = 0.0; int main () { int result = 0; if (sprintf (buf, "%F %d", 1234567.0, 33, 44, 55) < 0 || strcmp (buf, "1234567.000000 33") != 0) result |= 1; if (sprintf (buf, "%F", 1.0 / zero) < 0 || (strcmp (buf, "INF") != 0 && strcmp (buf, "INFINITY") != 0)) result |= 2; /* This catches a Cygwin 1.5.x bug. */ if (sprintf (buf, "%.F", 1234.0) < 0 || strcmp (buf, "1234") != 0) result |= 4; return result; }]])], [gl_cv_func_printf_directive_f=yes], [gl_cv_func_printf_directive_f=no], [ changequote(,)dnl case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_printf_directive_f="guessing yes";; # Guess yes on FreeBSD >= 6. freebsd[1-5].*) gl_cv_func_printf_directive_f="guessing no";; freebsd* | kfreebsd*) gl_cv_func_printf_directive_f="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_printf_directive_f="guessing no";; darwin*) gl_cv_func_printf_directive_f="guessing yes";; # Guess yes on Solaris >= 2.10. solaris2.[1-9][0-9]*) gl_cv_func_printf_sizes_c99="guessing yes";; solaris*) gl_cv_func_printf_sizes_c99="guessing no";; # If we don't know, assume the worst. *) gl_cv_func_printf_directive_f="guessing no";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions supports the %n format dnl directive. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_printf_directive_n. AC_DEFUN([gl_PRINTF_DIRECTIVE_N], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports the 'n' directive], [gl_cv_func_printf_directive_n], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include #ifdef _MSC_VER /* See page about "Parameter Validation" on msdn.microsoft.com. */ static void cdecl invalid_parameter_handler (const wchar_t *expression, const wchar_t *function, const wchar_t *file, unsigned int line, uintptr_t dummy) { exit (1); } #endif static char fmtstring[10]; static char buf[100]; int main () { int count = -1; #ifdef _MSC_VER _set_invalid_parameter_handler (invalid_parameter_handler); #endif /* Copy the format string. Some systems (glibc with _FORTIFY_SOURCE=2) support %n in format strings in read-only memory but not in writable memory. */ strcpy (fmtstring, "%d %n"); if (sprintf (buf, fmtstring, 123, &count, 33, 44, 55) < 0 || strcmp (buf, "123 ") != 0 || count != 4) return 1; return 0; }]])], [gl_cv_func_printf_directive_n=yes], [gl_cv_func_printf_directive_n=no], [ changequote(,)dnl case "$host_os" in mingw*) gl_cv_func_printf_directive_n="guessing no";; *) gl_cv_func_printf_directive_n="guessing yes";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions supports the %ls format dnl directive and in particular, when a precision is specified, whether dnl the functions stop converting the wide string argument when the number dnl of bytes that have been produced by this conversion equals or exceeds dnl the precision. dnl Result is gl_cv_func_printf_directive_ls. AC_DEFUN([gl_PRINTF_DIRECTIVE_LS], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports the 'ls' directive], [gl_cv_func_printf_directive_ls], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #include int main () { int result = 0; char buf[100]; /* Test whether %ls works at all. This test fails on OpenBSD 4.0, IRIX 6.5, Solaris 2.6, Haiku, but not on Cygwin 1.5. */ { static const wchar_t wstring[] = { 'a', 'b', 'c', 0 }; buf[0] = '\0'; if (sprintf (buf, "%ls", wstring) < 0 || strcmp (buf, "abc") != 0) result |= 1; } /* This test fails on IRIX 6.5, Solaris 2.6, Cygwin 1.5, Haiku (with an assertion failure inside libc), but not on OpenBSD 4.0. */ { static const wchar_t wstring[] = { 'a', 0 }; buf[0] = '\0'; if (sprintf (buf, "%ls", wstring) < 0 || strcmp (buf, "a") != 0) result |= 2; } /* Test whether precisions in %ls are supported as specified in ISO C 99 section 7.19.6.1: "If a precision is specified, no more than that many bytes are written (including shift sequences, if any), and the array shall contain a null wide character if, to equal the multibyte character sequence length given by the precision, the function would need to access a wide character one past the end of the array." This test fails on Solaris 10. */ { static const wchar_t wstring[] = { 'a', 'b', (wchar_t) 0xfdfdfdfd, 0 }; buf[0] = '\0'; if (sprintf (buf, "%.2ls", wstring) < 0 || strcmp (buf, "ab") != 0) result |= 8; } return result; }]])], [gl_cv_func_printf_directive_ls=yes], [gl_cv_func_printf_directive_ls=no], [ changequote(,)dnl case "$host_os" in openbsd*) gl_cv_func_printf_directive_ls="guessing no";; irix*) gl_cv_func_printf_directive_ls="guessing no";; solaris*) gl_cv_func_printf_directive_ls="guessing no";; cygwin*) gl_cv_func_printf_directive_ls="guessing no";; beos* | haiku*) gl_cv_func_printf_directive_ls="guessing no";; *) gl_cv_func_printf_directive_ls="guessing yes";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions supports POSIX/XSI format dnl strings with positions. (POSIX:2001) dnl Result is gl_cv_func_printf_positions. AC_DEFUN([gl_PRINTF_POSITIONS], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports POSIX/XSI format strings with positions], [gl_cv_func_printf_positions], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* The string "%2$d %1$d", with dollar characters protected from the shell's dollar expansion (possibly an autoconf bug). */ static char format[] = { '%', '2', '$', 'd', ' ', '%', '1', '$', 'd', '\0' }; static char buf[100]; int main () { sprintf (buf, format, 33, 55); return (strcmp (buf, "55 33") != 0); }]])], [gl_cv_func_printf_positions=yes], [gl_cv_func_printf_positions=no], [ changequote(,)dnl case "$host_os" in netbsd[1-3]* | netbsdelf[1-3]* | netbsdaout[1-3]* | netbsdcoff[1-3]*) gl_cv_func_printf_positions="guessing no";; beos*) gl_cv_func_printf_positions="guessing no";; mingw* | pw*) gl_cv_func_printf_positions="guessing no";; *) gl_cv_func_printf_positions="guessing yes";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions supports POSIX/XSI format dnl strings with the ' flag for grouping of decimal digits. (POSIX:2001) dnl Result is gl_cv_func_printf_flag_grouping. AC_DEFUN([gl_PRINTF_FLAG_GROUPING], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports the grouping flag], [gl_cv_func_printf_flag_grouping], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static char buf[100]; int main () { if (sprintf (buf, "%'d %d", 1234567, 99) < 0 || buf[strlen (buf) - 1] != '9') return 1; return 0; }]])], [gl_cv_func_printf_flag_grouping=yes], [gl_cv_func_printf_flag_grouping=no], [ changequote(,)dnl case "$host_os" in cygwin*) gl_cv_func_printf_flag_grouping="guessing no";; netbsd*) gl_cv_func_printf_flag_grouping="guessing no";; mingw* | pw*) gl_cv_func_printf_flag_grouping="guessing no";; *) gl_cv_func_printf_flag_grouping="guessing yes";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions supports the - flag correctly. dnl (ISO C99.) See dnl dnl Result is gl_cv_func_printf_flag_leftadjust. AC_DEFUN([gl_PRINTF_FLAG_LEFTADJUST], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports the left-adjust flag correctly], [gl_cv_func_printf_flag_leftadjust], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static char buf[100]; int main () { /* Check that a '-' flag is not annihilated by a negative width. */ if (sprintf (buf, "a%-*sc", -3, "b") < 0 || strcmp (buf, "ab c") != 0) return 1; return 0; }]])], [gl_cv_func_printf_flag_leftadjust=yes], [gl_cv_func_printf_flag_leftadjust=no], [ changequote(,)dnl case "$host_os" in # Guess yes on HP-UX 11. hpux11*) gl_cv_func_printf_flag_leftadjust="guessing yes";; # Guess no on HP-UX 10 and older. hpux*) gl_cv_func_printf_flag_leftadjust="guessing no";; # Guess yes otherwise. *) gl_cv_func_printf_flag_leftadjust="guessing yes";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions supports padding of non-finite dnl values with the 0 flag correctly. (ISO C99 + TC1 + TC2.) See dnl dnl Result is gl_cv_func_printf_flag_zero. AC_DEFUN([gl_PRINTF_FLAG_ZERO], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports the zero flag correctly], [gl_cv_func_printf_flag_zero], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static char buf[100]; static double zero = 0.0; int main () { if (sprintf (buf, "%010f", 1.0 / zero, 33, 44, 55) < 0 || (strcmp (buf, " inf") != 0 && strcmp (buf, " infinity") != 0)) return 1; return 0; }]])], [gl_cv_func_printf_flag_zero=yes], [gl_cv_func_printf_flag_zero=no], [ changequote(,)dnl case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_printf_flag_zero="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_printf_flag_zero="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_printf_flag_zero="guessing no";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions supports large precisions. dnl On mingw, precisions larger than 512 are treated like 512, in integer, dnl floating-point or pointer output. On Solaris 10/x86, precisions larger dnl than 510 in floating-point output crash the program. On Solaris 10/SPARC, dnl precisions larger than 510 in floating-point output yield wrong results. dnl On AIX 7.1, precisions larger than 998 in floating-point output yield dnl wrong results. On BeOS, precisions larger than 1044 crash the program. dnl Result is gl_cv_func_printf_precision. AC_DEFUN([gl_PRINTF_PRECISION], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports large precisions], [gl_cv_func_printf_precision], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static char buf[5000]; int main () { int result = 0; #ifdef __BEOS__ /* On BeOS, this would crash and show a dialog box. Avoid the crash. */ return 1; #endif if (sprintf (buf, "%.4000d %d", 1, 33, 44) < 4000 + 3) result |= 1; if (sprintf (buf, "%.4000f %d", 1.0, 33, 44) < 4000 + 5) result |= 2; if (sprintf (buf, "%.511f %d", 1.0, 33, 44) < 511 + 5 || buf[0] != '1') result |= 4; if (sprintf (buf, "%.999f %d", 1.0, 33, 44) < 999 + 5 || buf[0] != '1') result |= 4; return result; }]])], [gl_cv_func_printf_precision=yes], [gl_cv_func_printf_precision=no], [ changequote(,)dnl case "$host_os" in # Guess no only on Solaris, native Windows, and BeOS systems. solaris*) gl_cv_func_printf_precision="guessing no" ;; mingw* | pw*) gl_cv_func_printf_precision="guessing no" ;; beos*) gl_cv_func_printf_precision="guessing no" ;; *) gl_cv_func_printf_precision="guessing yes" ;; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions recovers gracefully in case dnl of an out-of-memory condition, or whether it crashes the entire program. dnl Result is gl_cv_func_printf_enomem. AC_DEFUN([gl_PRINTF_ENOMEM], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gl_MULTIARCH]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf survives out-of-memory conditions], [gl_cv_func_printf_enomem], [ gl_cv_func_printf_enomem="guessing no" if test "$cross_compiling" = no; then if test $APPLE_UNIVERSAL_BUILD = 0; then AC_LANG_CONFTEST([AC_LANG_SOURCE([ ]GL_NOCRASH[ changequote(,)dnl #include #include #include #include #include int main() { struct rlimit limit; int ret; nocrash_init (); /* Some printf implementations allocate temporary space with malloc. */ /* On BSD systems, malloc() is limited by RLIMIT_DATA. */ #ifdef RLIMIT_DATA if (getrlimit (RLIMIT_DATA, &limit) < 0) return 77; if (limit.rlim_max == RLIM_INFINITY || limit.rlim_max > 5000000) limit.rlim_max = 5000000; limit.rlim_cur = limit.rlim_max; if (setrlimit (RLIMIT_DATA, &limit) < 0) return 77; #endif /* On Linux systems, malloc() is limited by RLIMIT_AS. */ #ifdef RLIMIT_AS if (getrlimit (RLIMIT_AS, &limit) < 0) return 77; if (limit.rlim_max == RLIM_INFINITY || limit.rlim_max > 5000000) limit.rlim_max = 5000000; limit.rlim_cur = limit.rlim_max; if (setrlimit (RLIMIT_AS, &limit) < 0) return 77; #endif /* Some printf implementations allocate temporary space on the stack. */ #ifdef RLIMIT_STACK if (getrlimit (RLIMIT_STACK, &limit) < 0) return 77; if (limit.rlim_max == RLIM_INFINITY || limit.rlim_max > 5000000) limit.rlim_max = 5000000; limit.rlim_cur = limit.rlim_max; if (setrlimit (RLIMIT_STACK, &limit) < 0) return 77; #endif ret = printf ("%.5000000f", 1.0); return !(ret == 5000002 || (ret < 0 && errno == ENOMEM)); } changequote([,])dnl ])]) if AC_TRY_EVAL([ac_link]) && test -s conftest$ac_exeext; then (./conftest 2>&AS_MESSAGE_LOG_FD result=$? _AS_ECHO_LOG([\$? = $result]) if test $result != 0 && test $result != 77; then result=1; fi exit $result ) >/dev/null 2>/dev/null case $? in 0) gl_cv_func_printf_enomem="yes" ;; 77) gl_cv_func_printf_enomem="guessing no" ;; *) gl_cv_func_printf_enomem="no" ;; esac else gl_cv_func_printf_enomem="guessing no" fi rm -fr conftest* else dnl A universal build on Apple Mac OS X platforms. dnl The result would be 'no' in 32-bit mode and 'yes' in 64-bit mode. dnl But we need a configuration result that is valid in both modes. gl_cv_func_printf_enomem="guessing no" fi fi if test "$gl_cv_func_printf_enomem" = "guessing no"; then changequote(,)dnl case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_printf_enomem="guessing yes";; # Guess yes on Solaris. solaris*) gl_cv_func_printf_enomem="guessing yes";; # Guess yes on AIX. aix*) gl_cv_func_printf_enomem="guessing yes";; # Guess yes on HP-UX/hppa. hpux*) case "$host_cpu" in hppa*) gl_cv_func_printf_enomem="guessing yes";; *) gl_cv_func_printf_enomem="guessing no";; esac ;; # Guess yes on IRIX. irix*) gl_cv_func_printf_enomem="guessing yes";; # Guess yes on OSF/1. osf*) gl_cv_func_printf_enomem="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_printf_enomem="guessing yes";; # Guess yes on Haiku. haiku*) gl_cv_func_printf_enomem="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_printf_enomem="guessing no";; esac changequote([,])dnl fi ]) ]) dnl Test whether the snprintf function exists. (ISO C99, POSIX:2001) dnl Result is ac_cv_func_snprintf. AC_DEFUN([gl_SNPRINTF_PRESENCE], [ AC_CHECK_FUNCS_ONCE([snprintf]) ]) dnl Test whether the string produced by the snprintf function is always NUL dnl terminated. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_snprintf_truncation_c99. AC_DEFUN([gl_SNPRINTF_TRUNCATION_C99], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_SNPRINTF_PRESENCE]) AC_CACHE_CHECK([whether snprintf truncates the result as in C99], [gl_cv_func_snprintf_truncation_c99], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #if HAVE_SNPRINTF # define my_snprintf snprintf #else # include static int my_snprintf (char *buf, int size, const char *format, ...) { va_list args; int ret; va_start (args, format); ret = vsnprintf (buf, size, format, args); va_end (args); return ret; } #endif static char buf[100]; int main () { strcpy (buf, "ABCDEF"); my_snprintf (buf, 3, "%d %d", 4567, 89); if (memcmp (buf, "45\0DEF", 6) != 0) return 1; return 0; }]])], [gl_cv_func_snprintf_truncation_c99=yes], [gl_cv_func_snprintf_truncation_c99=no], [ changequote(,)dnl case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on FreeBSD >= 5. freebsd[1-4].*) gl_cv_func_snprintf_truncation_c99="guessing no";; freebsd* | kfreebsd*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_snprintf_truncation_c99="guessing no";; darwin*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on OpenBSD >= 3.9. openbsd[1-2].* | openbsd3.[0-8] | openbsd3.[0-8].*) gl_cv_func_snprintf_truncation_c99="guessing no";; openbsd*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on Solaris >= 2.6. solaris2.[0-5] | solaris2.[0-5].*) gl_cv_func_snprintf_truncation_c99="guessing no";; solaris*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on AIX >= 4. aix[1-3]*) gl_cv_func_snprintf_truncation_c99="guessing no";; aix*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on HP-UX >= 11. hpux[7-9]* | hpux10*) gl_cv_func_snprintf_truncation_c99="guessing no";; hpux*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on IRIX >= 6.5. irix6.5) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on OSF/1 >= 5. osf[3-4]*) gl_cv_func_snprintf_truncation_c99="guessing no";; osf*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on NetBSD >= 3. netbsd[1-2]* | netbsdelf[1-2]* | netbsdaout[1-2]* | netbsdcoff[1-2]*) gl_cv_func_snprintf_truncation_c99="guessing no";; netbsd*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_snprintf_truncation_c99="guessing no";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the return value of the snprintf function is the number dnl of bytes (excluding the terminating NUL) that would have been produced dnl if the buffer had been large enough. (ISO C99, POSIX:2001) dnl For example, this test program fails on IRIX 6.5: dnl --------------------------------------------------------------------- dnl #include dnl int main() dnl { dnl static char buf[8]; dnl int retval = snprintf (buf, 3, "%d", 12345); dnl return retval >= 0 && retval < 3; dnl } dnl --------------------------------------------------------------------- dnl Result is gl_cv_func_snprintf_retval_c99. AC_DEFUN_ONCE([gl_SNPRINTF_RETVAL_C99], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_SNPRINTF_PRESENCE]) AC_CACHE_CHECK([whether snprintf returns a byte count as in C99], [gl_cv_func_snprintf_retval_c99], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #if HAVE_SNPRINTF # define my_snprintf snprintf #else # include static int my_snprintf (char *buf, int size, const char *format, ...) { va_list args; int ret; va_start (args, format); ret = vsnprintf (buf, size, format, args); va_end (args); return ret; } #endif static char buf[100]; int main () { strcpy (buf, "ABCDEF"); if (my_snprintf (buf, 3, "%d %d", 4567, 89) != 7) return 1; if (my_snprintf (buf, 0, "%d %d", 4567, 89) != 7) return 2; if (my_snprintf (NULL, 0, "%d %d", 4567, 89) != 7) return 3; return 0; }]])], [gl_cv_func_snprintf_retval_c99=yes], [gl_cv_func_snprintf_retval_c99=no], [ changequote(,)dnl case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on FreeBSD >= 5. freebsd[1-4].*) gl_cv_func_snprintf_retval_c99="guessing no";; freebsd* | kfreebsd*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_snprintf_retval_c99="guessing no";; darwin*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on OpenBSD >= 3.9. openbsd[1-2].* | openbsd3.[0-8] | openbsd3.[0-8].*) gl_cv_func_snprintf_retval_c99="guessing no";; openbsd*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on Solaris >= 2.10. solaris2.[1-9][0-9]*) gl_cv_func_printf_sizes_c99="guessing yes";; solaris*) gl_cv_func_printf_sizes_c99="guessing no";; # Guess yes on AIX >= 4. aix[1-3]*) gl_cv_func_snprintf_retval_c99="guessing no";; aix*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on NetBSD >= 3. netbsd[1-2]* | netbsdelf[1-2]* | netbsdaout[1-2]* | netbsdcoff[1-2]*) gl_cv_func_snprintf_retval_c99="guessing no";; netbsd*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_snprintf_retval_c99="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_snprintf_retval_c99="guessing no";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the snprintf function supports the %n format directive dnl also in truncated portions of the format string. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_snprintf_directive_n. AC_DEFUN([gl_SNPRINTF_DIRECTIVE_N], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_SNPRINTF_PRESENCE]) AC_CACHE_CHECK([whether snprintf fully supports the 'n' directive], [gl_cv_func_snprintf_directive_n], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #if HAVE_SNPRINTF # define my_snprintf snprintf #else # include static int my_snprintf (char *buf, int size, const char *format, ...) { va_list args; int ret; va_start (args, format); ret = vsnprintf (buf, size, format, args); va_end (args); return ret; } #endif static char fmtstring[10]; static char buf[100]; int main () { int count = -1; /* Copy the format string. Some systems (glibc with _FORTIFY_SOURCE=2) support %n in format strings in read-only memory but not in writable memory. */ strcpy (fmtstring, "%d %n"); my_snprintf (buf, 4, fmtstring, 12345, &count, 33, 44, 55); if (count != 6) return 1; return 0; }]])], [gl_cv_func_snprintf_directive_n=yes], [gl_cv_func_snprintf_directive_n=no], [ changequote(,)dnl case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on FreeBSD >= 5. freebsd[1-4].*) gl_cv_func_snprintf_directive_n="guessing no";; freebsd* | kfreebsd*) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_snprintf_directive_n="guessing no";; darwin*) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on Solaris >= 2.6. solaris2.[0-5] | solaris2.[0-5].*) gl_cv_func_snprintf_directive_n="guessing no";; solaris*) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on AIX >= 4. aix[1-3]*) gl_cv_func_snprintf_directive_n="guessing no";; aix*) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on IRIX >= 6.5. irix6.5) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on OSF/1 >= 5. osf[3-4]*) gl_cv_func_snprintf_directive_n="guessing no";; osf*) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on NetBSD >= 3. netbsd[1-2]* | netbsdelf[1-2]* | netbsdaout[1-2]* | netbsdcoff[1-2]*) gl_cv_func_snprintf_directive_n="guessing no";; netbsd*) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_snprintf_directive_n="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_snprintf_directive_n="guessing no";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the snprintf function, when passed a size = 1, writes any dnl output without bounds in this case, behaving like sprintf. This is the dnl case on Linux libc5. dnl Result is gl_cv_func_snprintf_size1. AC_DEFUN([gl_SNPRINTF_SIZE1], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gl_SNPRINTF_PRESENCE]) AC_CACHE_CHECK([whether snprintf respects a size of 1], [gl_cv_func_snprintf_size1], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #if HAVE_SNPRINTF # define my_snprintf snprintf #else # include static int my_snprintf (char *buf, int size, const char *format, ...) { va_list args; int ret; va_start (args, format); ret = vsnprintf (buf, size, format, args); va_end (args); return ret; } #endif int main() { static char buf[8] = { 'D', 'E', 'A', 'D', 'B', 'E', 'E', 'F' }; my_snprintf (buf, 1, "%d", 12345); return buf[1] != 'E'; }]])], [gl_cv_func_snprintf_size1=yes], [gl_cv_func_snprintf_size1=no], [gl_cv_func_snprintf_size1="guessing yes"]) ]) ]) dnl Test whether the vsnprintf function, when passed a zero size, produces no dnl output. (ISO C99, POSIX:2001) dnl For example, snprintf nevertheless writes a NUL byte in this case dnl on OSF/1 5.1: dnl --------------------------------------------------------------------- dnl #include dnl int main() dnl { dnl static char buf[8] = { 'D', 'E', 'A', 'D', 'B', 'E', 'E', 'F' }; dnl snprintf (buf, 0, "%d", 12345); dnl return buf[0] != 'D'; dnl } dnl --------------------------------------------------------------------- dnl And vsnprintf writes any output without bounds in this case, behaving like dnl vsprintf, on HP-UX 11 and OSF/1 5.1: dnl --------------------------------------------------------------------- dnl #include dnl #include dnl static int my_snprintf (char *buf, int size, const char *format, ...) dnl { dnl va_list args; dnl int ret; dnl va_start (args, format); dnl ret = vsnprintf (buf, size, format, args); dnl va_end (args); dnl return ret; dnl } dnl int main() dnl { dnl static char buf[8] = { 'D', 'E', 'A', 'D', 'B', 'E', 'E', 'F' }; dnl my_snprintf (buf, 0, "%d", 12345); dnl return buf[0] != 'D'; dnl } dnl --------------------------------------------------------------------- dnl Result is gl_cv_func_vsnprintf_zerosize_c99. AC_DEFUN([gl_VSNPRINTF_ZEROSIZE_C99], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether vsnprintf respects a zero size as in C99], [gl_cv_func_vsnprintf_zerosize_c99], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static int my_snprintf (char *buf, int size, const char *format, ...) { va_list args; int ret; va_start (args, format); ret = vsnprintf (buf, size, format, args); va_end (args); return ret; } int main() { static char buf[8] = { 'D', 'E', 'A', 'D', 'B', 'E', 'E', 'F' }; my_snprintf (buf, 0, "%d", 12345); return buf[0] != 'D'; }]])], [gl_cv_func_vsnprintf_zerosize_c99=yes], [gl_cv_func_vsnprintf_zerosize_c99=no], [ changequote(,)dnl case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on FreeBSD >= 5. freebsd[1-4].*) gl_cv_func_vsnprintf_zerosize_c99="guessing no";; freebsd* | kfreebsd*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_vsnprintf_zerosize_c99="guessing no";; darwin*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on Cygwin. cygwin*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on Solaris >= 2.6. solaris2.[0-5] | solaris2.[0-5].*) gl_cv_func_vsnprintf_zerosize_c99="guessing no";; solaris*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on AIX >= 4. aix[1-3]*) gl_cv_func_vsnprintf_zerosize_c99="guessing no";; aix*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on IRIX >= 6.5. irix6.5) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on NetBSD >= 3. netbsd[1-2]* | netbsdelf[1-2]* | netbsdaout[1-2]* | netbsdcoff[1-2]*) gl_cv_func_vsnprintf_zerosize_c99="guessing no";; netbsd*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on mingw. mingw* | pw*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_vsnprintf_zerosize_c99="guessing no";; esac changequote([,])dnl ]) ]) ]) dnl The results of these tests on various platforms are: dnl dnl 1 = gl_PRINTF_SIZES_C99 dnl 2 = gl_PRINTF_LONG_DOUBLE dnl 3 = gl_PRINTF_INFINITE dnl 4 = gl_PRINTF_INFINITE_LONG_DOUBLE dnl 5 = gl_PRINTF_DIRECTIVE_A dnl 6 = gl_PRINTF_DIRECTIVE_F dnl 7 = gl_PRINTF_DIRECTIVE_N dnl 8 = gl_PRINTF_DIRECTIVE_LS dnl 9 = gl_PRINTF_POSITIONS dnl 10 = gl_PRINTF_FLAG_GROUPING dnl 11 = gl_PRINTF_FLAG_LEFTADJUST dnl 12 = gl_PRINTF_FLAG_ZERO dnl 13 = gl_PRINTF_PRECISION dnl 14 = gl_PRINTF_ENOMEM dnl 15 = gl_SNPRINTF_PRESENCE dnl 16 = gl_SNPRINTF_TRUNCATION_C99 dnl 17 = gl_SNPRINTF_RETVAL_C99 dnl 18 = gl_SNPRINTF_DIRECTIVE_N dnl 19 = gl_SNPRINTF_SIZE1 dnl 20 = gl_VSNPRINTF_ZEROSIZE_C99 dnl dnl 1 = checking whether printf supports size specifiers as in C99... dnl 2 = checking whether printf supports 'long double' arguments... dnl 3 = checking whether printf supports infinite 'double' arguments... dnl 4 = checking whether printf supports infinite 'long double' arguments... dnl 5 = checking whether printf supports the 'a' and 'A' directives... dnl 6 = checking whether printf supports the 'F' directive... dnl 7 = checking whether printf supports the 'n' directive... dnl 8 = checking whether printf supports the 'ls' directive... dnl 9 = checking whether printf supports POSIX/XSI format strings with positions... dnl 10 = checking whether printf supports the grouping flag... dnl 11 = checking whether printf supports the left-adjust flag correctly... dnl 12 = checking whether printf supports the zero flag correctly... dnl 13 = checking whether printf supports large precisions... dnl 14 = checking whether printf survives out-of-memory conditions... dnl 15 = checking for snprintf... dnl 16 = checking whether snprintf truncates the result as in C99... dnl 17 = checking whether snprintf returns a byte count as in C99... dnl 18 = checking whether snprintf fully supports the 'n' directive... dnl 19 = checking whether snprintf respects a size of 1... dnl 20 = checking whether vsnprintf respects a zero size as in C99... dnl dnl . = yes, # = no. dnl dnl 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 dnl glibc 2.5 . . . . . . . . . . . . . . . . . . . . dnl glibc 2.3.6 . . . . # . . . . . . . . . . . . . . . dnl FreeBSD 5.4, 6.1 . . . . # . . . . . . # . # . . . . . . dnl Mac OS X 10.5.8 . . . # # . . . . . . # . . . . . . . . dnl Mac OS X 10.3.9 . . . . # . . . . . . # . # . . . . . . dnl OpenBSD 3.9, 4.0 . . # # # # . # . # . # . # . . . . . . dnl Cygwin 1.7.0 (2009) . . . # . . . ? . . . . . ? . . . . . . dnl Cygwin 1.5.25 (2008) . . . # # . . # . . . . . # . . . . . . dnl Cygwin 1.5.19 (2006) # . . # # # . # . # . # # # . . . . . . dnl Solaris 11 2011-11 . . # # # . . # . . . # . . . . . . . . dnl Solaris 10 . . # # # . . # . . . # # . . . . . . . dnl Solaris 2.6 ... 9 # . # # # # . # . . . # # . . . # . . . dnl Solaris 2.5.1 # . # # # # . # . . . # . . # # # # # # dnl AIX 7.1 . . # # # . . . . . . # # . . . . . . . dnl AIX 5.2 . . # # # . . . . . . # . . . . . . . . dnl AIX 4.3.2, 5.1 # . # # # # . . . . . # . . . . # . . . dnl HP-UX 11.31 . . . . # . . . . . . # . . . . # # . . dnl HP-UX 11.{00,11,23} # . . . # # . . . . . # . . . . # # . # dnl HP-UX 10.20 # . # . # # . ? . . # # . . . . # # ? # dnl IRIX 6.5 # . # # # # . # . . . # . . . . # . . . dnl OSF/1 5.1 # . # # # # . . . . . # . . . . # . . # dnl OSF/1 4.0d # . # # # # . . . . . # . . # # # # # # dnl NetBSD 5.0 . . . # # . . . . . . # . # . . . . . . dnl NetBSD 4.0 . ? ? ? ? ? . ? . ? ? ? ? ? . . . ? ? ? dnl NetBSD 3.0 . . . . # # . ? # # ? # . # . . . . . . dnl Haiku . . . # # # . # . . . . . ? . . ? . . . dnl BeOS # # . # # # . ? # . ? . # ? . . ? . . . dnl old mingw / msvcrt # # # # # # . . # # . # # ? . # # # . . dnl MSVC 9 # # # # # # # . # # . # # ? # # # # . . dnl mingw 2009-2011 . # . # . . . . # # . . . ? . . . . . . dnl mingw-w64 2011 # # # # # # . . # # . # # ? . # # # . . gnuastro-0.2.33-8a3b/bootstrapped/m4/pathmax.m40000644000175000017500000000220413004436755016054 00000000000000# pathmax.m4 serial 10 dnl Copyright (C) 2002-2003, 2005-2006, 2009-2016 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_PATHMAX], [ dnl Prerequisites of lib/pathmax.h. AC_CHECK_HEADERS_ONCE([sys/param.h]) ]) # Expands to a piece of C program that defines PATH_MAX in the same way as # "pathmax.h" will do. AC_DEFUN([gl_PATHMAX_SNIPPET], [[ /* Arrange to define PATH_MAX, like "pathmax.h" does. */ #if HAVE_UNISTD_H # include #endif #include #if defined HAVE_SYS_PARAM_H && !defined PATH_MAX && !defined MAXPATHLEN # include #endif #if !defined PATH_MAX && defined MAXPATHLEN # define PATH_MAX MAXPATHLEN #endif #ifdef __hpux # undef PATH_MAX # define PATH_MAX 1024 #endif #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # undef PATH_MAX # define PATH_MAX 260 #endif ]]) # Prerequisites of gl_PATHMAX_SNIPPET. AC_DEFUN([gl_PATHMAX_SNIPPET_PREREQ], [ AC_CHECK_HEADERS_ONCE([unistd.h sys/param.h]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/open.m40000644000175000017500000000504613004436755015362 00000000000000# open.m4 serial 14 dnl Copyright (C) 2007-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_OPEN], [ AC_REQUIRE([AC_CANONICAL_HOST]) case "$host_os" in mingw* | pw*) REPLACE_OPEN=1 ;; *) dnl open("foo/") should not create a file when the file name has a dnl trailing slash. FreeBSD only has the problem on symlinks. AC_CHECK_FUNCS_ONCE([lstat]) AC_CACHE_CHECK([whether open recognizes a trailing slash], [gl_cv_func_open_slash], [# Assume that if we have lstat, we can also check symlinks. if test $ac_cv_func_lstat = yes; then touch conftest.tmp ln -s conftest.tmp conftest.lnk fi AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #if HAVE_UNISTD_H # include #endif int main () { int result = 0; #if HAVE_LSTAT if (open ("conftest.lnk/", O_RDONLY) != -1) result |= 1; #endif if (open ("conftest.sl/", O_CREAT, 0600) >= 0) result |= 2; return result; }]])], [gl_cv_func_open_slash=yes], [gl_cv_func_open_slash=no], [ changequote(,)dnl case "$host_os" in freebsd* | aix* | hpux* | solaris2.[0-9] | solaris2.[0-9].*) gl_cv_func_open_slash="guessing no" ;; *) gl_cv_func_open_slash="guessing yes" ;; esac changequote([,])dnl ]) rm -f conftest.sl conftest.tmp conftest.lnk ]) case "$gl_cv_func_open_slash" in *no) AC_DEFINE([OPEN_TRAILING_SLASH_BUG], [1], [Define to 1 if open() fails to recognize a trailing slash.]) REPLACE_OPEN=1 ;; esac ;; esac dnl Replace open() for supporting the gnulib-defined fchdir() function, dnl to keep fchdir's bookkeeping up-to-date. m4_ifdef([gl_FUNC_FCHDIR], [ if test $REPLACE_OPEN = 0; then gl_TEST_FCHDIR if test $HAVE_FCHDIR = 0; then REPLACE_OPEN=1 fi fi ]) dnl Replace open() for supporting the gnulib-defined O_NONBLOCK flag. m4_ifdef([gl_NONBLOCKING_IO], [ if test $REPLACE_OPEN = 0; then gl_NONBLOCKING_IO if test $gl_cv_have_open_O_NONBLOCK != yes; then REPLACE_OPEN=1 fi fi ]) ]) # Prerequisites of lib/open.c. AC_DEFUN([gl_PREREQ_OPEN], [ AC_REQUIRE([gl_PROMOTED_TYPE_MODE_T]) : ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/off_t.m40000644000175000017500000000100613004436755015506 00000000000000# off_t.m4 serial 1 dnl Copyright (C) 2012-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Check whether to override the 'off_t' type. dnl Set WINDOWS_64_BIT_OFF_T. AC_DEFUN([gl_TYPE_OFF_T], [ m4_ifdef([gl_LARGEFILE], [ AC_REQUIRE([gl_LARGEFILE]) ], [ WINDOWS_64_BIT_OFF_T=0 ]) AC_SUBST([WINDOWS_64_BIT_OFF_T]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/nproc.m40000644000175000017500000000347013004436755015541 00000000000000# nproc.m4 serial 5 dnl Copyright (C) 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_NPROC], [ gl_PREREQ_NPROC ]) # Prerequisites of lib/nproc.c. AC_DEFUN([gl_PREREQ_NPROC], [ dnl Persuade glibc to declare CPU_SETSIZE, CPU_ISSET etc. AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_CHECK_HEADERS([sys/pstat.h sys/sysmp.h sys/param.h],,, [AC_INCLUDES_DEFAULT]) dnl requires on OpenBSD 4.0. AC_CHECK_HEADERS([sys/sysctl.h],,, [AC_INCLUDES_DEFAULT #if HAVE_SYS_PARAM_H # include #endif ]) AC_CHECK_FUNCS([sched_getaffinity sched_getaffinity_np \ pstat_getdynamic sysmp sysctl]) dnl Test whether sched_getaffinity has the expected declaration. dnl glibc 2.3.[0-2]: dnl int sched_getaffinity (pid_t, unsigned int, unsigned long int *); dnl glibc 2.3.3: dnl int sched_getaffinity (pid_t, cpu_set_t *); dnl glibc >= 2.3.4: dnl int sched_getaffinity (pid_t, size_t, cpu_set_t *); if test $ac_cv_func_sched_getaffinity = yes; then AC_CACHE_CHECK([for glibc compatible sched_getaffinity], [gl_cv_func_sched_getaffinity3], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include #include ]], [[sched_getaffinity (0, 0, (cpu_set_t *) 0);]])], [gl_cv_func_sched_getaffinity3=yes], [gl_cv_func_sched_getaffinity3=no]) ]) if test $gl_cv_func_sched_getaffinity3 = yes; then AC_DEFINE([HAVE_SCHED_GETAFFINITY_LIKE_GLIBC], [1], [Define to 1 if sched_getaffinity has a glibc compatible declaration.]) fi fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/nocrash.m40000644000175000017500000001060213004436755016050 00000000000000# nocrash.m4 serial 4 dnl Copyright (C) 2005, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Based on libsigsegv, from Bruno Haible and Paolo Bonzini. AC_PREREQ([2.13]) dnl Expands to some code for use in .c programs that will cause the configure dnl test to exit instead of crashing. This is useful to avoid triggering dnl action from a background debugger and to avoid core dumps. dnl Usage: ... dnl ]GL_NOCRASH[ dnl ... dnl int main() { nocrash_init(); ... } AC_DEFUN([GL_NOCRASH],[[ #include #if defined __MACH__ && defined __APPLE__ /* Avoid a crash on Mac OS X. */ #include #include #include #include #include #include /* The exception port on which our thread listens. */ static mach_port_t our_exception_port; /* The main function of the thread listening for exceptions of type EXC_BAD_ACCESS. */ static void * mach_exception_thread (void *arg) { /* Buffer for a message to be received. */ struct { mach_msg_header_t head; mach_msg_body_t msgh_body; char data[1024]; } msg; mach_msg_return_t retval; /* Wait for a message on the exception port. */ retval = mach_msg (&msg.head, MACH_RCV_MSG | MACH_RCV_LARGE, 0, sizeof (msg), our_exception_port, MACH_MSG_TIMEOUT_NONE, MACH_PORT_NULL); if (retval != MACH_MSG_SUCCESS) abort (); exit (1); } static void nocrash_init (void) { mach_port_t self = mach_task_self (); /* Allocate a port on which the thread shall listen for exceptions. */ if (mach_port_allocate (self, MACH_PORT_RIGHT_RECEIVE, &our_exception_port) == KERN_SUCCESS) { /* See http://web.mit.edu/darwin/src/modules/xnu/osfmk/man/mach_port_insert_right.html. */ if (mach_port_insert_right (self, our_exception_port, our_exception_port, MACH_MSG_TYPE_MAKE_SEND) == KERN_SUCCESS) { /* The exceptions we want to catch. Only EXC_BAD_ACCESS is interesting for us. */ exception_mask_t mask = EXC_MASK_BAD_ACCESS; /* Create the thread listening on the exception port. */ pthread_attr_t attr; pthread_t thread; if (pthread_attr_init (&attr) == 0 && pthread_attr_setdetachstate (&attr, PTHREAD_CREATE_DETACHED) == 0 && pthread_create (&thread, &attr, mach_exception_thread, NULL) == 0) { pthread_attr_destroy (&attr); /* Replace the exception port info for these exceptions with our own. Note that we replace the exception port for the entire task, not only for a particular thread. This has the effect that when our exception port gets the message, the thread specific exception port has already been asked, and we don't need to bother about it. See http://web.mit.edu/darwin/src/modules/xnu/osfmk/man/task_set_exception_ports.html. */ task_set_exception_ports (self, mask, our_exception_port, EXCEPTION_DEFAULT, MACHINE_THREAD_STATE); } } } } #elif (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Avoid a crash on native Windows. */ #define WIN32_LEAN_AND_MEAN #include #include static LONG WINAPI exception_filter (EXCEPTION_POINTERS *ExceptionInfo) { switch (ExceptionInfo->ExceptionRecord->ExceptionCode) { case EXCEPTION_ACCESS_VIOLATION: case EXCEPTION_IN_PAGE_ERROR: case EXCEPTION_STACK_OVERFLOW: case EXCEPTION_GUARD_PAGE: case EXCEPTION_PRIV_INSTRUCTION: case EXCEPTION_ILLEGAL_INSTRUCTION: case EXCEPTION_DATATYPE_MISALIGNMENT: case EXCEPTION_ARRAY_BOUNDS_EXCEEDED: case EXCEPTION_NONCONTINUABLE_EXCEPTION: exit (1); } return EXCEPTION_CONTINUE_SEARCH; } static void nocrash_init (void) { SetUnhandledExceptionFilter ((LPTOP_LEVEL_EXCEPTION_FILTER) exception_filter); } #else /* Avoid a crash on POSIX systems. */ #include #include /* A POSIX signal handler. */ static void exception_handler (int sig) { _exit (1); } static void nocrash_init (void) { #ifdef SIGSEGV signal (SIGSEGV, exception_handler); #endif #ifdef SIGBUS signal (SIGBUS, exception_handler); #endif } #endif ]]) gnuastro-0.2.33-8a3b/bootstrapped/m4/nl_langinfo.m40000644000175000017500000000352413004436755016706 00000000000000# nl_langinfo.m4 serial 5 dnl Copyright (C) 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_NL_LANGINFO], [ AC_REQUIRE([gl_LANGINFO_H_DEFAULTS]) AC_REQUIRE([gl_LANGINFO_H]) AC_CHECK_FUNCS_ONCE([nl_langinfo]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles if test $ac_cv_func_nl_langinfo = yes; then # On Irix 6.5, YESEXPR is defined, but nl_langinfo(YESEXPR) is broken. AC_CACHE_CHECK([whether YESEXPR works], [gl_cv_func_nl_langinfo_yesexpr_works], [AC_RUN_IFELSE( [AC_LANG_PROGRAM([[#include ]], [[return !*nl_langinfo(YESEXPR); ]])], [gl_cv_func_nl_langinfo_yesexpr_works=yes], [gl_cv_func_nl_langinfo_yesexpr_works=no], [ case "$host_os" in # Guess no on irix systems. irix*) gl_cv_func_nl_langinfo_yesexpr_works="guessing no";; # Guess yes elsewhere. *) gl_cv_func_nl_langinfo_yesexpr_works="guessing yes";; esac ]) ]) case $gl_cv_func_nl_langinfo_yesexpr_works in *yes) FUNC_NL_LANGINFO_YESEXPR_WORKS=1 ;; *) FUNC_NL_LANGINFO_YESEXPR_WORKS=0 ;; esac AC_DEFINE_UNQUOTED([FUNC_NL_LANGINFO_YESEXPR_WORKS], [$FUNC_NL_LANGINFO_YESEXPR_WORKS], [Define to 1 if nl_langinfo (YESEXPR) returns a non-empty string.]) if test $HAVE_LANGINFO_CODESET = 1 && test $HAVE_LANGINFO_ERA = 1 \ && test $FUNC_NL_LANGINFO_YESEXPR_WORKS = 1; then : else REPLACE_NL_LANGINFO=1 AC_DEFINE([REPLACE_NL_LANGINFO], [1], [Define if nl_langinfo exists but is overridden by gnulib.]) fi else HAVE_NL_LANGINFO=0 fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/multiarch.m40000644000175000017500000000367413004436755016416 00000000000000# multiarch.m4 serial 7 dnl Copyright (C) 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # Determine whether the compiler is or may be producing universal binaries. # # On Mac OS X 10.5 and later systems, the user can create libraries and # executables that work on multiple system types--known as "fat" or # "universal" binaries--by specifying multiple '-arch' options to the # compiler but only a single '-arch' option to the preprocessor. Like # this: # # ./configure CC="gcc -arch i386 -arch x86_64 -arch ppc -arch ppc64" \ # CXX="g++ -arch i386 -arch x86_64 -arch ppc -arch ppc64" \ # CPP="gcc -E" CXXCPP="g++ -E" # # Detect this situation and set APPLE_UNIVERSAL_BUILD accordingly. AC_DEFUN_ONCE([gl_MULTIARCH], [ dnl Code similar to autoconf-2.63 AC_C_BIGENDIAN. gl_cv_c_multiarch=no AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#ifndef __APPLE_CC__ not a universal capable compiler #endif typedef int dummy; ]])], [ dnl Check for potential -arch flags. It is not universal unless dnl there are at least two -arch flags with different values. arch= prev= for word in ${CC} ${CFLAGS} ${CPPFLAGS} ${LDFLAGS}; do if test -n "$prev"; then case $word in i?86 | x86_64 | ppc | ppc64) if test -z "$arch" || test "$arch" = "$word"; then arch="$word" else gl_cv_c_multiarch=yes fi ;; esac prev= else if test "x$word" = "x-arch"; then prev=arch fi fi done ]) if test $gl_cv_c_multiarch = yes; then APPLE_UNIVERSAL_BUILD=1 else APPLE_UNIVERSAL_BUILD=0 fi AC_SUBST([APPLE_UNIVERSAL_BUILD]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/msvc-nothrow.m40000644000175000017500000000053013004436755017060 00000000000000# msvc-nothrow.m4 serial 1 dnl Copyright (C) 2011-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_MSVC_NOTHROW], [ AC_REQUIRE([gl_MSVC_INVAL]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/msvc-inval.m40000644000175000017500000000133413004436755016474 00000000000000# msvc-inval.m4 serial 1 dnl Copyright (C) 2011-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_MSVC_INVAL], [ AC_CHECK_FUNCS_ONCE([_set_invalid_parameter_handler]) if test $ac_cv_func__set_invalid_parameter_handler = yes; then HAVE_MSVC_INVALID_PARAMETER_HANDLER=1 AC_DEFINE([HAVE_MSVC_INVALID_PARAMETER_HANDLER], [1], [Define to 1 on MSVC platforms that have the "invalid parameter handler" concept.]) else HAVE_MSVC_INVALID_PARAMETER_HANDLER=0 fi AC_SUBST([HAVE_MSVC_INVALID_PARAMETER_HANDLER]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/mode_t.m40000644000175000017500000000234213004436755015664 00000000000000# mode_t.m4 serial 2 dnl Copyright (C) 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # For using mode_t, it's sufficient to use AC_TYPE_MODE_T and # include . # Define PROMOTED_MODE_T to the type that is the result of "default argument # promotion" (ISO C 6.5.2.2.(6)) of the type mode_t. AC_DEFUN([gl_PROMOTED_TYPE_MODE_T], [ AC_REQUIRE([AC_TYPE_MODE_T]) AC_CACHE_CHECK([for promoted mode_t type], [gl_cv_promoted_mode_t], [ dnl Assume mode_t promotes to 'int' if and only if it is smaller than 'int', dnl and to itself otherwise. This assumption is not guaranteed by the ISO C dnl standard, but we don't know of any real-world counterexamples. AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[#include ]], [[typedef int array[2 * (sizeof (mode_t) < sizeof (int)) - 1];]])], [gl_cv_promoted_mode_t='int'], [gl_cv_promoted_mode_t='mode_t']) ]) AC_DEFINE_UNQUOTED([PROMOTED_MODE_T], [$gl_cv_promoted_mode_t], [Define to the type that is the result of default argument promotions of type mode_t.]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/mmap-anon.m40000644000175000017500000000373313004436755016305 00000000000000# mmap-anon.m4 serial 10 dnl Copyright (C) 2005, 2007, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # Detect how mmap can be used to create anonymous (not file-backed) memory # mappings. # - On Linux, AIX, OSF/1, Solaris, Cygwin, Interix, Haiku, both MAP_ANONYMOUS # and MAP_ANON exist and have the same value. # - On HP-UX, only MAP_ANONYMOUS exists. # - On Mac OS X, FreeBSD, NetBSD, OpenBSD, only MAP_ANON exists. # - On IRIX, neither exists, and a file descriptor opened to /dev/zero must be # used. AC_DEFUN([gl_FUNC_MMAP_ANON], [ dnl Persuade glibc to define MAP_ANONYMOUS. AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) # Check for mmap(). Don't use AC_FUNC_MMAP, because it checks too much: it # fails on HP-UX 11, because MAP_FIXED mappings do not work. But this is # irrelevant for anonymous mappings. AC_CHECK_FUNC([mmap], [gl_have_mmap=yes], [gl_have_mmap=no]) # Try to allow MAP_ANONYMOUS. gl_have_mmap_anonymous=no if test $gl_have_mmap = yes; then AC_MSG_CHECKING([for MAP_ANONYMOUS]) AC_EGREP_CPP([I cannot identify this map], [ #include #ifdef MAP_ANONYMOUS I cannot identify this map #endif ], [gl_have_mmap_anonymous=yes]) if test $gl_have_mmap_anonymous != yes; then AC_EGREP_CPP([I cannot identify this map], [ #include #ifdef MAP_ANON I cannot identify this map #endif ], [AC_DEFINE([MAP_ANONYMOUS], [MAP_ANON], [Define to a substitute value for mmap()'s MAP_ANONYMOUS flag.]) gl_have_mmap_anonymous=yes]) fi AC_MSG_RESULT([$gl_have_mmap_anonymous]) if test $gl_have_mmap_anonymous = yes; then AC_DEFINE([HAVE_MAP_ANONYMOUS], [1], [Define to 1 if mmap()'s MAP_ANONYMOUS flag is available after including config.h and .]) fi fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/mempcpy.m40000644000175000017500000000134613004436755016072 00000000000000# mempcpy.m4 serial 11 dnl Copyright (C) 2003-2004, 2006-2007, 2009-2016 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_MEMPCPY], [ dnl Persuade glibc to declare mempcpy(). AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) dnl The mempcpy() declaration in lib/string.in.h uses 'restrict'. AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) AC_CHECK_FUNCS([mempcpy]) if test $ac_cv_func_mempcpy = no; then HAVE_MEMPCPY=0 fi ]) # Prerequisites of lib/mempcpy.c. AC_DEFUN([gl_PREREQ_MEMPCPY], [ : ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/memchr.m40000644000175000017500000000534013004436755015671 00000000000000# memchr.m4 serial 12 dnl Copyright (C) 2002-2004, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN_ONCE([gl_FUNC_MEMCHR], [ dnl Check for prerequisites for memory fence checks. gl_FUNC_MMAP_ANON AC_CHECK_HEADERS_ONCE([sys/mman.h]) AC_CHECK_FUNCS_ONCE([mprotect]) AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) m4_ifdef([gl_FUNC_MEMCHR_OBSOLETE], [ dnl These days, we assume memchr is present. But if support for old dnl platforms is desired: AC_CHECK_FUNCS_ONCE([memchr]) if test $ac_cv_func_memchr = no; then HAVE_MEMCHR=0 fi ]) if test $HAVE_MEMCHR = 1; then # Detect platform-specific bugs in some versions of glibc: # memchr should not dereference anything with length 0 # http://bugzilla.redhat.com/499689 # memchr should not dereference overestimated length after a match # http://bugs.debian.org/cgi-bin/bugreport.cgi?bug=521737 # http://sourceware.org/bugzilla/show_bug.cgi?id=10162 # Assume that memchr works on platforms that lack mprotect. AC_CACHE_CHECK([whether memchr works], [gl_cv_func_memchr_works], [AC_RUN_IFELSE([AC_LANG_PROGRAM([[ #include #if HAVE_SYS_MMAN_H # include # include # include # include # ifndef MAP_FILE # define MAP_FILE 0 # endif #endif ]], [[ int result = 0; char *fence = NULL; #if HAVE_SYS_MMAN_H && HAVE_MPROTECT # if HAVE_MAP_ANONYMOUS const int flags = MAP_ANONYMOUS | MAP_PRIVATE; const int fd = -1; # else /* !HAVE_MAP_ANONYMOUS */ const int flags = MAP_FILE | MAP_PRIVATE; int fd = open ("/dev/zero", O_RDONLY, 0666); if (fd >= 0) # endif { int pagesize = getpagesize (); char *two_pages = (char *) mmap (NULL, 2 * pagesize, PROT_READ | PROT_WRITE, flags, fd, 0); if (two_pages != (char *)(-1) && mprotect (two_pages + pagesize, pagesize, PROT_NONE) == 0) fence = two_pages + pagesize; } #endif if (fence) { if (memchr (fence, 0, 0)) result |= 1; strcpy (fence - 9, "12345678"); if (memchr (fence - 9, 0, 79) != fence - 1) result |= 2; if (memchr (fence - 1, 0, 3) != fence - 1) result |= 4; } return result; ]])], [gl_cv_func_memchr_works=yes], [gl_cv_func_memchr_works=no], [dnl Be pessimistic for now. gl_cv_func_memchr_works="guessing no"])]) if test "$gl_cv_func_memchr_works" != yes; then REPLACE_MEMCHR=1 fi fi ]) # Prerequisites of lib/memchr.c. AC_DEFUN([gl_PREREQ_MEMCHR], [ AC_CHECK_HEADERS([bp-sym.h]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/mbtowc.m40000644000175000017500000000071413004436755015711 00000000000000# mbtowc.m4 serial 2 dnl Copyright (C) 2011-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_MBTOWC], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) if false; then REPLACE_MBTOWC=1 fi ]) # Prerequisites of lib/mbtowc.c. AC_DEFUN([gl_PREREQ_MBTOWC], [ : ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/mbstate_t.m40000644000175000017500000000256713004436755016410 00000000000000# mbstate_t.m4 serial 13 dnl Copyright (C) 2000-2002, 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # From Paul Eggert. # BeOS 5 has but does not define mbstate_t, # so you can't declare an object of that type. # Check for this incompatibility with Standard C. # AC_TYPE_MBSTATE_T # ----------------- AC_DEFUN([AC_TYPE_MBSTATE_T], [ AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) dnl for HP-UX 11.11 AC_CACHE_CHECK([for mbstate_t], [ac_cv_type_mbstate_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [AC_INCLUDES_DEFAULT[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include ]], [[mbstate_t x; return sizeof x;]])], [ac_cv_type_mbstate_t=yes], [ac_cv_type_mbstate_t=no])]) if test $ac_cv_type_mbstate_t = yes; then AC_DEFINE([HAVE_MBSTATE_T], [1], [Define to 1 if declares mbstate_t.]) else AC_DEFINE([mbstate_t], [int], [Define to a type if does not define.]) fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/mbsinit.m40000644000175000017500000000276313004436755016071 00000000000000# mbsinit.m4 serial 8 dnl Copyright (C) 2008, 2010-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_MBSINIT], [ AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([AC_TYPE_MBSTATE_T]) gl_MBSTATE_T_BROKEN AC_CHECK_FUNCS_ONCE([mbsinit]) if test $ac_cv_func_mbsinit = no; then HAVE_MBSINIT=0 AC_CHECK_DECLS([mbsinit],,, [[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include ]]) if test $ac_cv_have_decl_mbsinit = yes; then dnl On Minix 3.1.8, the system's declares mbsinit() although dnl it does not have the function. Avoid a collision with gnulib's dnl replacement. REPLACE_MBSINIT=1 fi else if test $REPLACE_MBSTATE_T = 1; then REPLACE_MBSINIT=1 else dnl On mingw, mbsinit() always returns 1, which is inappropriate for dnl states produced by mbrtowc() for an incomplete multibyte character dnl in multibyte locales. case "$host_os" in mingw*) REPLACE_MBSINIT=1 ;; esac fi fi ]) # Prerequisites of lib/mbsinit.c. AC_DEFUN([gl_PREREQ_MBSINIT], [ : ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/mbrtowc.m40000644000175000017500000004725013004436755016101 00000000000000# mbrtowc.m4 serial 27 -*- coding: utf-8 -*- dnl Copyright (C) 2001-2002, 2004-2005, 2008-2016 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_MBRTOWC], [ AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) AC_REQUIRE([AC_TYPE_MBSTATE_T]) gl_MBSTATE_T_BROKEN AC_CHECK_FUNCS_ONCE([mbrtowc]) if test $ac_cv_func_mbrtowc = no; then HAVE_MBRTOWC=0 AC_CHECK_DECLS([mbrtowc],,, [[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include ]]) if test $ac_cv_have_decl_mbrtowc = yes; then dnl On Minix 3.1.8, the system's declares mbrtowc() although dnl it does not have the function. Avoid a collision with gnulib's dnl replacement. REPLACE_MBRTOWC=1 fi else if test $REPLACE_MBSTATE_T = 1; then REPLACE_MBRTOWC=1 else gl_MBRTOWC_NULL_ARG1 gl_MBRTOWC_NULL_ARG2 gl_MBRTOWC_RETVAL gl_MBRTOWC_NUL_RETVAL gl_MBRTOWC_EMPTY_INPUT gl_MBRTOWC_C_LOCALE case "$gl_cv_func_mbrtowc_null_arg1" in *yes) ;; *) AC_DEFINE([MBRTOWC_NULL_ARG1_BUG], [1], [Define if the mbrtowc function has the NULL pwc argument bug.]) REPLACE_MBRTOWC=1 ;; esac case "$gl_cv_func_mbrtowc_null_arg2" in *yes) ;; *) AC_DEFINE([MBRTOWC_NULL_ARG2_BUG], [1], [Define if the mbrtowc function has the NULL string argument bug.]) REPLACE_MBRTOWC=1 ;; esac case "$gl_cv_func_mbrtowc_retval" in *yes) ;; *) AC_DEFINE([MBRTOWC_RETVAL_BUG], [1], [Define if the mbrtowc function returns a wrong return value.]) REPLACE_MBRTOWC=1 ;; esac case "$gl_cv_func_mbrtowc_nul_retval" in *yes) ;; *) AC_DEFINE([MBRTOWC_NUL_RETVAL_BUG], [1], [Define if the mbrtowc function does not return 0 for a NUL character.]) REPLACE_MBRTOWC=1 ;; esac case "$gl_cv_func_mbrtowc_empty_input" in *yes) ;; *) AC_DEFINE([MBRTOWC_EMPTY_INPUT_BUG], [1], [Define if the mbrtowc function does not return (size_t) -2 for empty input.]) REPLACE_MBRTOWC=1 ;; esac case $gl_cv_C_locale_sans_EILSEQ in *yes) ;; *) AC_DEFINE([C_LOCALE_MAYBE_EILSEQ], [1], [Define to 1 if the C locale may have encoding errors.]) REPLACE_MBRTOWC=1 ;; esac fi fi ]) dnl Test whether mbsinit() and mbrtowc() need to be overridden in a way that dnl redefines the semantics of the given mbstate_t type. dnl Result is REPLACE_MBSTATE_T. dnl When this is set to 1, we replace both mbsinit() and mbrtowc(), in order to dnl avoid inconsistencies. AC_DEFUN([gl_MBSTATE_T_BROKEN], [ AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) AC_REQUIRE([AC_TYPE_MBSTATE_T]) AC_CHECK_FUNCS_ONCE([mbsinit]) AC_CHECK_FUNCS_ONCE([mbrtowc]) if test $ac_cv_func_mbsinit = yes && test $ac_cv_func_mbrtowc = yes; then gl_MBRTOWC_INCOMPLETE_STATE gl_MBRTOWC_SANITYCHECK REPLACE_MBSTATE_T=0 case "$gl_cv_func_mbrtowc_incomplete_state" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac case "$gl_cv_func_mbrtowc_sanitycheck" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac else REPLACE_MBSTATE_T=1 fi ]) dnl Test whether mbrtowc puts the state into non-initial state when parsing an dnl incomplete multibyte character. dnl Result is gl_cv_func_mbrtowc_incomplete_state. AC_DEFUN([gl_MBRTOWC_INCOMPLETE_STATE], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_JA]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether mbrtowc handles incomplete characters], [gl_cv_func_mbrtowc_incomplete_state], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on AIX and OSF/1. aix* | osf*) gl_cv_func_mbrtowc_incomplete_state="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_incomplete_state="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_JA != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { const char input[] = "B\217\253\344\217\251\316er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) if (mbsinit (&state)) return 1; } return 0; }]])], [gl_cv_func_mbrtowc_incomplete_state=yes], [gl_cv_func_mbrtowc_incomplete_state=no], [:]) fi ]) ]) dnl Test whether mbrtowc works not worse than mbtowc. dnl Result is gl_cv_func_mbrtowc_sanitycheck. AC_DEFUN([gl_MBRTOWC_SANITYCHECK], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_ZH_CN]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether mbrtowc works as well as mbtowc], [gl_cv_func_mbrtowc_sanitycheck], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on Solaris 8. solaris2.8) gl_cv_func_mbrtowc_sanitycheck="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_sanitycheck="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_ZH_CN != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { /* This fails on Solaris 8: mbrtowc returns 2, and sets wc to 0x00F0. mbtowc returns 4 (correct) and sets wc to 0x5EDC. */ if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { char input[] = "B\250\271\201\060\211\070er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 6, &state) != 4 && mbtowc (&wc, input + 3, 6) == 4) return 1; } return 0; }]])], [gl_cv_func_mbrtowc_sanitycheck=yes], [gl_cv_func_mbrtowc_sanitycheck=no], [:]) fi ]) ]) dnl Test whether mbrtowc supports a NULL pwc argument correctly. dnl Result is gl_cv_func_mbrtowc_null_arg1. AC_DEFUN([gl_MBRTOWC_NULL_ARG1], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_FR_UTF8]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether mbrtowc handles a NULL pwc argument], [gl_cv_func_mbrtowc_null_arg1], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on Solaris. solaris*) gl_cv_func_mbrtowc_null_arg1="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_null_arg1="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_FR_UTF8 != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { int result = 0; if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { char input[] = "\303\237er"; mbstate_t state; wchar_t wc; size_t ret; memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 5, &state); if (ret != 2) result |= 1; if (!mbsinit (&state)) result |= 2; memset (&state, '\0', sizeof (mbstate_t)); ret = mbrtowc (NULL, input, 5, &state); if (ret != 2) /* Solaris 7 fails here: ret is -1. */ result |= 4; if (!mbsinit (&state)) result |= 8; } return result; }]])], [gl_cv_func_mbrtowc_null_arg1=yes], [gl_cv_func_mbrtowc_null_arg1=no], [:]) fi ]) ]) dnl Test whether mbrtowc supports a NULL string argument correctly. dnl Result is gl_cv_func_mbrtowc_null_arg2. AC_DEFUN([gl_MBRTOWC_NULL_ARG2], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_FR_UTF8]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether mbrtowc handles a NULL string argument], [gl_cv_func_mbrtowc_null_arg2], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on OSF/1. osf*) gl_cv_func_mbrtowc_null_arg2="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_null_arg2="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_FR_UTF8 != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { mbstate_t state; wchar_t wc; int ret; memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; mbrtowc (&wc, NULL, 5, &state); /* Check that wc was not modified. */ if (wc != (wchar_t) 0xBADFACE) return 1; } return 0; }]])], [gl_cv_func_mbrtowc_null_arg2=yes], [gl_cv_func_mbrtowc_null_arg2=no], [:]) fi ]) ]) dnl Test whether mbrtowc, when parsing the end of a multibyte character, dnl correctly returns the number of bytes that were needed to complete the dnl character (not the total number of bytes of the multibyte character). dnl Result is gl_cv_func_mbrtowc_retval. AC_DEFUN([gl_MBRTOWC_RETVAL], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_FR_UTF8]) AC_REQUIRE([gt_LOCALE_JA]) AC_REQUIRE([AC_CANONICAL_HOST]) AC_CACHE_CHECK([whether mbrtowc has a correct return value], [gl_cv_func_mbrtowc_retval], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on HP-UX, Solaris, native Windows. hpux* | solaris* | mingw*) gl_cv_func_mbrtowc_retval="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_retval="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_FR_UTF8 != none || test $LOCALE_JA != none \ || { case "$host_os" in mingw*) true;; *) false;; esac; }; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { int result = 0; int found_some_locale = 0; /* This fails on Solaris. */ if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { char input[] = "B\303\274\303\237er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) { input[1] = '\0'; if (mbrtowc (&wc, input + 2, 5, &state) != 1) result |= 1; } found_some_locale = 1; } /* This fails on HP-UX 11.11. */ if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { char input[] = "B\217\253\344\217\251\316er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) { input[1] = '\0'; if (mbrtowc (&wc, input + 2, 5, &state) != 2) result |= 2; } found_some_locale = 1; } /* This fails on native Windows. */ if (setlocale (LC_ALL, "Japanese_Japan.932") != NULL) { char input[] = "<\223\372\226\173\214\352>"; /* "<日本語>" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 1, &state) == (size_t)(-2)) { input[3] = '\0'; if (mbrtowc (&wc, input + 4, 4, &state) != 1) result |= 4; } found_some_locale = 1; } if (setlocale (LC_ALL, "Chinese_Taiwan.950") != NULL) { char input[] = "<\244\351\245\273\273\171>"; /* "<日本語>" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 1, &state) == (size_t)(-2)) { input[3] = '\0'; if (mbrtowc (&wc, input + 4, 4, &state) != 1) result |= 8; } found_some_locale = 1; } if (setlocale (LC_ALL, "Chinese_China.936") != NULL) { char input[] = "<\310\325\261\276\325\132>"; /* "<日本語>" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 1, &state) == (size_t)(-2)) { input[3] = '\0'; if (mbrtowc (&wc, input + 4, 4, &state) != 1) result |= 16; } found_some_locale = 1; } return (found_some_locale ? result : 77); }]])], [gl_cv_func_mbrtowc_retval=yes], [if test $? != 77; then gl_cv_func_mbrtowc_retval=no fi ], [:]) fi ]) ]) dnl Test whether mbrtowc, when parsing a NUL character, correctly returns 0. dnl Result is gl_cv_func_mbrtowc_nul_retval. AC_DEFUN([gl_MBRTOWC_NUL_RETVAL], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_ZH_CN]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether mbrtowc returns 0 when parsing a NUL character], [gl_cv_func_mbrtowc_nul_retval], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on Solaris 8 and 9. solaris2.[89]) gl_cv_func_mbrtowc_nul_retval="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_nul_retval="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_ZH_CN != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { /* This fails on Solaris 8 and 9. */ if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, "", 1, &state) != 0) return 1; } return 0; }]])], [gl_cv_func_mbrtowc_nul_retval=yes], [gl_cv_func_mbrtowc_nul_retval=no], [:]) fi ]) ]) dnl Test whether mbrtowc returns the correct value on empty input. AC_DEFUN([gl_MBRTOWC_EMPTY_INPUT], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether mbrtowc works on empty input], [gl_cv_func_mbrtowc_empty_input], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on AIX and glibc systems. aix* | *-gnu*) gl_cv_func_mbrtowc_empty_input="guessing no" ;; *) gl_cv_func_mbrtowc_empty_input="guessing yes" ;; esac changequote([,])dnl AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include static wchar_t wc; static mbstate_t mbs; int main (void) { return mbrtowc (&wc, "", 0, &mbs) != (size_t) -2; }]])], [gl_cv_func_mbrtowc_empty_input=yes], [gl_cv_func_mbrtowc_empty_input=no], [:]) ]) ]) dnl Test whether mbrtowc reports encoding errors in the C locale. dnl Although POSIX was never intended to allow this, the GNU C Library dnl and other implementations do it. See: dnl https://sourceware.org/bugzilla/show_bug.cgi?id=19932 AC_DEFUN([gl_MBRTOWC_C_LOCALE], [ AC_CACHE_CHECK([whether the C locale is free of encoding errors], [gl_cv_C_locale_sans_EILSEQ], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. gl_cv_C_locale_sans_EILSEQ="guessing no" AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include #include ]], [[ int i; char *locale = setlocale (LC_ALL, "C"); if (! locale) return 1; for (i = CHAR_MIN; i <= CHAR_MAX; i++) { char c = i; wchar_t wc; mbstate_t mbs = { 0, }; size_t ss = mbrtowc (&wc, &c, 1, &mbs); if (1 < ss) return 1; } return 0; ]])], [gl_cv_C_locale_sans_EILSEQ=yes], [gl_cv_C_locale_sans_EILSEQ=no], [:])]) ]) # Prerequisites of lib/mbrtowc.c. AC_DEFUN([gl_PREREQ_MBRTOWC], [ : ]) dnl From Paul Eggert dnl This is an override of an autoconf macro. AC_DEFUN([AC_FUNC_MBRTOWC], [ dnl Same as AC_FUNC_MBRTOWC in autoconf-2.60. AC_CACHE_CHECK([whether mbrtowc and mbstate_t are properly declared], gl_cv_func_mbrtowc, [AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[/* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include ]], [[wchar_t wc; char const s[] = ""; size_t n = 1; mbstate_t state; return ! (sizeof state && (mbrtowc) (&wc, s, n, &state));]])], gl_cv_func_mbrtowc=yes, gl_cv_func_mbrtowc=no)]) if test $gl_cv_func_mbrtowc = yes; then AC_DEFINE([HAVE_MBRTOWC], [1], [Define to 1 if mbrtowc and mbstate_t are properly declared.]) fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/math_h.m40000644000175000017500000004211113004436755015653 00000000000000# math_h.m4 serial 114 dnl Copyright (C) 2007-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_MATH_H], [ AC_REQUIRE([gl_MATH_H_DEFAULTS]) gl_CHECK_NEXT_HEADERS([math.h]) AC_CACHE_CHECK([whether NAN macro works], [gl_cv_header_math_nan_works], [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[@%:@include ]], [[/* Solaris 10 has a broken definition of NAN. Other platforms fail to provide NAN, or provide it only in C99 mode; this test only needs to fail when NAN is provided but wrong. */ float f = 1.0f; #ifdef NAN f = NAN; #endif return f == 0;]])], [gl_cv_header_math_nan_works=yes], [gl_cv_header_math_nan_works=no])]) if test $gl_cv_header_math_nan_works = no; then REPLACE_NAN=1 fi AC_CACHE_CHECK([whether HUGE_VAL works], [gl_cv_header_math_huge_val_works], [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[@%:@include ]], [[/* Solaris 10 has a broken definition of HUGE_VAL. */ double d = HUGE_VAL; return d == 0;]])], [gl_cv_header_math_huge_val_works=yes], [gl_cv_header_math_huge_val_works=no])]) if test $gl_cv_header_math_huge_val_works = no; then REPLACE_HUGE_VAL=1 fi dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[#include ]], [acosf acosl asinf asinl atanf atanl cbrt cbrtf cbrtl ceilf ceill copysign copysignf copysignl cosf cosl coshf expf expl exp2 exp2f exp2l expm1 expm1f expm1l fabsf fabsl floorf floorl fma fmaf fmal fmod fmodf fmodl frexpf frexpl hypotf hypotl ilogb ilogbf ilogbl ldexpf ldexpl log logf logl log10 log10f log10l log1p log1pf log1pl log2 log2f log2l logb logbf logbl modf modff modfl powf remainder remainderf remainderl rint rintf rintl round roundf roundl sinf sinl sinhf sqrtf sqrtl tanf tanl tanhf trunc truncf truncl]) ]) AC_DEFUN([gl_MATH_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_MATH_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_MATH_H_DEFAULTS], [ GNULIB_ACOSF=0; AC_SUBST([GNULIB_ACOSF]) GNULIB_ACOSL=0; AC_SUBST([GNULIB_ACOSL]) GNULIB_ASINF=0; AC_SUBST([GNULIB_ASINF]) GNULIB_ASINL=0; AC_SUBST([GNULIB_ASINL]) GNULIB_ATANF=0; AC_SUBST([GNULIB_ATANF]) GNULIB_ATANL=0; AC_SUBST([GNULIB_ATANL]) GNULIB_ATAN2F=0; AC_SUBST([GNULIB_ATAN2F]) GNULIB_CBRT=0; AC_SUBST([GNULIB_CBRT]) GNULIB_CBRTF=0; AC_SUBST([GNULIB_CBRTF]) GNULIB_CBRTL=0; AC_SUBST([GNULIB_CBRTL]) GNULIB_CEIL=0; AC_SUBST([GNULIB_CEIL]) GNULIB_CEILF=0; AC_SUBST([GNULIB_CEILF]) GNULIB_CEILL=0; AC_SUBST([GNULIB_CEILL]) GNULIB_COPYSIGN=0; AC_SUBST([GNULIB_COPYSIGN]) GNULIB_COPYSIGNF=0; AC_SUBST([GNULIB_COPYSIGNF]) GNULIB_COPYSIGNL=0; AC_SUBST([GNULIB_COPYSIGNL]) GNULIB_COSF=0; AC_SUBST([GNULIB_COSF]) GNULIB_COSL=0; AC_SUBST([GNULIB_COSL]) GNULIB_COSHF=0; AC_SUBST([GNULIB_COSHF]) GNULIB_EXPF=0; AC_SUBST([GNULIB_EXPF]) GNULIB_EXPL=0; AC_SUBST([GNULIB_EXPL]) GNULIB_EXP2=0; AC_SUBST([GNULIB_EXP2]) GNULIB_EXP2F=0; AC_SUBST([GNULIB_EXP2F]) GNULIB_EXP2L=0; AC_SUBST([GNULIB_EXP2L]) GNULIB_EXPM1=0; AC_SUBST([GNULIB_EXPM1]) GNULIB_EXPM1F=0; AC_SUBST([GNULIB_EXPM1F]) GNULIB_EXPM1L=0; AC_SUBST([GNULIB_EXPM1L]) GNULIB_FABSF=0; AC_SUBST([GNULIB_FABSF]) GNULIB_FABSL=0; AC_SUBST([GNULIB_FABSL]) GNULIB_FLOOR=0; AC_SUBST([GNULIB_FLOOR]) GNULIB_FLOORF=0; AC_SUBST([GNULIB_FLOORF]) GNULIB_FLOORL=0; AC_SUBST([GNULIB_FLOORL]) GNULIB_FMA=0; AC_SUBST([GNULIB_FMA]) GNULIB_FMAF=0; AC_SUBST([GNULIB_FMAF]) GNULIB_FMAL=0; AC_SUBST([GNULIB_FMAL]) GNULIB_FMOD=0; AC_SUBST([GNULIB_FMOD]) GNULIB_FMODF=0; AC_SUBST([GNULIB_FMODF]) GNULIB_FMODL=0; AC_SUBST([GNULIB_FMODL]) GNULIB_FREXPF=0; AC_SUBST([GNULIB_FREXPF]) GNULIB_FREXP=0; AC_SUBST([GNULIB_FREXP]) GNULIB_FREXPL=0; AC_SUBST([GNULIB_FREXPL]) GNULIB_HYPOT=0; AC_SUBST([GNULIB_HYPOT]) GNULIB_HYPOTF=0; AC_SUBST([GNULIB_HYPOTF]) GNULIB_HYPOTL=0; AC_SUBST([GNULIB_HYPOTL]) GNULIB_ILOGB=0; AC_SUBST([GNULIB_ILOGB]) GNULIB_ILOGBF=0; AC_SUBST([GNULIB_ILOGBF]) GNULIB_ILOGBL=0; AC_SUBST([GNULIB_ILOGBL]) GNULIB_ISFINITE=0; AC_SUBST([GNULIB_ISFINITE]) GNULIB_ISINF=0; AC_SUBST([GNULIB_ISINF]) GNULIB_ISNAN=0; AC_SUBST([GNULIB_ISNAN]) GNULIB_ISNANF=0; AC_SUBST([GNULIB_ISNANF]) GNULIB_ISNAND=0; AC_SUBST([GNULIB_ISNAND]) GNULIB_ISNANL=0; AC_SUBST([GNULIB_ISNANL]) GNULIB_LDEXPF=0; AC_SUBST([GNULIB_LDEXPF]) GNULIB_LDEXPL=0; AC_SUBST([GNULIB_LDEXPL]) GNULIB_LOG=0; AC_SUBST([GNULIB_LOG]) GNULIB_LOGF=0; AC_SUBST([GNULIB_LOGF]) GNULIB_LOGL=0; AC_SUBST([GNULIB_LOGL]) GNULIB_LOG10=0; AC_SUBST([GNULIB_LOG10]) GNULIB_LOG10F=0; AC_SUBST([GNULIB_LOG10F]) GNULIB_LOG10L=0; AC_SUBST([GNULIB_LOG10L]) GNULIB_LOG1P=0; AC_SUBST([GNULIB_LOG1P]) GNULIB_LOG1PF=0; AC_SUBST([GNULIB_LOG1PF]) GNULIB_LOG1PL=0; AC_SUBST([GNULIB_LOG1PL]) GNULIB_LOG2=0; AC_SUBST([GNULIB_LOG2]) GNULIB_LOG2F=0; AC_SUBST([GNULIB_LOG2F]) GNULIB_LOG2L=0; AC_SUBST([GNULIB_LOG2L]) GNULIB_LOGB=0; AC_SUBST([GNULIB_LOGB]) GNULIB_LOGBF=0; AC_SUBST([GNULIB_LOGBF]) GNULIB_LOGBL=0; AC_SUBST([GNULIB_LOGBL]) GNULIB_MODF=0; AC_SUBST([GNULIB_MODF]) GNULIB_MODFF=0; AC_SUBST([GNULIB_MODFF]) GNULIB_MODFL=0; AC_SUBST([GNULIB_MODFL]) GNULIB_POWF=0; AC_SUBST([GNULIB_POWF]) GNULIB_REMAINDER=0; AC_SUBST([GNULIB_REMAINDER]) GNULIB_REMAINDERF=0; AC_SUBST([GNULIB_REMAINDERF]) GNULIB_REMAINDERL=0; AC_SUBST([GNULIB_REMAINDERL]) GNULIB_RINT=0; AC_SUBST([GNULIB_RINT]) GNULIB_RINTF=0; AC_SUBST([GNULIB_RINTF]) GNULIB_RINTL=0; AC_SUBST([GNULIB_RINTL]) GNULIB_ROUND=0; AC_SUBST([GNULIB_ROUND]) GNULIB_ROUNDF=0; AC_SUBST([GNULIB_ROUNDF]) GNULIB_ROUNDL=0; AC_SUBST([GNULIB_ROUNDL]) GNULIB_SIGNBIT=0; AC_SUBST([GNULIB_SIGNBIT]) GNULIB_SINF=0; AC_SUBST([GNULIB_SINF]) GNULIB_SINL=0; AC_SUBST([GNULIB_SINL]) GNULIB_SINHF=0; AC_SUBST([GNULIB_SINHF]) GNULIB_SQRTF=0; AC_SUBST([GNULIB_SQRTF]) GNULIB_SQRTL=0; AC_SUBST([GNULIB_SQRTL]) GNULIB_TANF=0; AC_SUBST([GNULIB_TANF]) GNULIB_TANL=0; AC_SUBST([GNULIB_TANL]) GNULIB_TANHF=0; AC_SUBST([GNULIB_TANHF]) GNULIB_TRUNC=0; AC_SUBST([GNULIB_TRUNC]) GNULIB_TRUNCF=0; AC_SUBST([GNULIB_TRUNCF]) GNULIB_TRUNCL=0; AC_SUBST([GNULIB_TRUNCL]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_ACOSF=1; AC_SUBST([HAVE_ACOSF]) HAVE_ACOSL=1; AC_SUBST([HAVE_ACOSL]) HAVE_ASINF=1; AC_SUBST([HAVE_ASINF]) HAVE_ASINL=1; AC_SUBST([HAVE_ASINL]) HAVE_ATANF=1; AC_SUBST([HAVE_ATANF]) HAVE_ATANL=1; AC_SUBST([HAVE_ATANL]) HAVE_ATAN2F=1; AC_SUBST([HAVE_ATAN2F]) HAVE_CBRT=1; AC_SUBST([HAVE_CBRT]) HAVE_CBRTF=1; AC_SUBST([HAVE_CBRTF]) HAVE_CBRTL=1; AC_SUBST([HAVE_CBRTL]) HAVE_COPYSIGN=1; AC_SUBST([HAVE_COPYSIGN]) HAVE_COPYSIGNL=1; AC_SUBST([HAVE_COPYSIGNL]) HAVE_COSF=1; AC_SUBST([HAVE_COSF]) HAVE_COSL=1; AC_SUBST([HAVE_COSL]) HAVE_COSHF=1; AC_SUBST([HAVE_COSHF]) HAVE_EXPF=1; AC_SUBST([HAVE_EXPF]) HAVE_EXPL=1; AC_SUBST([HAVE_EXPL]) HAVE_EXPM1=1; AC_SUBST([HAVE_EXPM1]) HAVE_EXPM1F=1; AC_SUBST([HAVE_EXPM1F]) HAVE_FABSF=1; AC_SUBST([HAVE_FABSF]) HAVE_FABSL=1; AC_SUBST([HAVE_FABSL]) HAVE_FMA=1; AC_SUBST([HAVE_FMA]) HAVE_FMAF=1; AC_SUBST([HAVE_FMAF]) HAVE_FMAL=1; AC_SUBST([HAVE_FMAL]) HAVE_FMODF=1; AC_SUBST([HAVE_FMODF]) HAVE_FMODL=1; AC_SUBST([HAVE_FMODL]) HAVE_FREXPF=1; AC_SUBST([HAVE_FREXPF]) HAVE_HYPOTF=1; AC_SUBST([HAVE_HYPOTF]) HAVE_HYPOTL=1; AC_SUBST([HAVE_HYPOTL]) HAVE_ILOGB=1; AC_SUBST([HAVE_ILOGB]) HAVE_ILOGBF=1; AC_SUBST([HAVE_ILOGBF]) HAVE_ILOGBL=1; AC_SUBST([HAVE_ILOGBL]) HAVE_ISNANF=1; AC_SUBST([HAVE_ISNANF]) HAVE_ISNAND=1; AC_SUBST([HAVE_ISNAND]) HAVE_ISNANL=1; AC_SUBST([HAVE_ISNANL]) HAVE_LDEXPF=1; AC_SUBST([HAVE_LDEXPF]) HAVE_LOGF=1; AC_SUBST([HAVE_LOGF]) HAVE_LOGL=1; AC_SUBST([HAVE_LOGL]) HAVE_LOG10F=1; AC_SUBST([HAVE_LOG10F]) HAVE_LOG10L=1; AC_SUBST([HAVE_LOG10L]) HAVE_LOG1P=1; AC_SUBST([HAVE_LOG1P]) HAVE_LOG1PF=1; AC_SUBST([HAVE_LOG1PF]) HAVE_LOG1PL=1; AC_SUBST([HAVE_LOG1PL]) HAVE_LOGBF=1; AC_SUBST([HAVE_LOGBF]) HAVE_LOGBL=1; AC_SUBST([HAVE_LOGBL]) HAVE_MODFF=1; AC_SUBST([HAVE_MODFF]) HAVE_MODFL=1; AC_SUBST([HAVE_MODFL]) HAVE_POWF=1; AC_SUBST([HAVE_POWF]) HAVE_REMAINDER=1; AC_SUBST([HAVE_REMAINDER]) HAVE_REMAINDERF=1; AC_SUBST([HAVE_REMAINDERF]) HAVE_RINT=1; AC_SUBST([HAVE_RINT]) HAVE_RINTL=1; AC_SUBST([HAVE_RINTL]) HAVE_SINF=1; AC_SUBST([HAVE_SINF]) HAVE_SINL=1; AC_SUBST([HAVE_SINL]) HAVE_SINHF=1; AC_SUBST([HAVE_SINHF]) HAVE_SQRTF=1; AC_SUBST([HAVE_SQRTF]) HAVE_SQRTL=1; AC_SUBST([HAVE_SQRTL]) HAVE_TANF=1; AC_SUBST([HAVE_TANF]) HAVE_TANL=1; AC_SUBST([HAVE_TANL]) HAVE_TANHF=1; AC_SUBST([HAVE_TANHF]) HAVE_DECL_ACOSL=1; AC_SUBST([HAVE_DECL_ACOSL]) HAVE_DECL_ASINL=1; AC_SUBST([HAVE_DECL_ASINL]) HAVE_DECL_ATANL=1; AC_SUBST([HAVE_DECL_ATANL]) HAVE_DECL_CBRTF=1; AC_SUBST([HAVE_DECL_CBRTF]) HAVE_DECL_CBRTL=1; AC_SUBST([HAVE_DECL_CBRTL]) HAVE_DECL_CEILF=1; AC_SUBST([HAVE_DECL_CEILF]) HAVE_DECL_CEILL=1; AC_SUBST([HAVE_DECL_CEILL]) HAVE_DECL_COPYSIGNF=1; AC_SUBST([HAVE_DECL_COPYSIGNF]) HAVE_DECL_COSL=1; AC_SUBST([HAVE_DECL_COSL]) HAVE_DECL_EXPL=1; AC_SUBST([HAVE_DECL_EXPL]) HAVE_DECL_EXP2=1; AC_SUBST([HAVE_DECL_EXP2]) HAVE_DECL_EXP2F=1; AC_SUBST([HAVE_DECL_EXP2F]) HAVE_DECL_EXP2L=1; AC_SUBST([HAVE_DECL_EXP2L]) HAVE_DECL_EXPM1L=1; AC_SUBST([HAVE_DECL_EXPM1L]) HAVE_DECL_FLOORF=1; AC_SUBST([HAVE_DECL_FLOORF]) HAVE_DECL_FLOORL=1; AC_SUBST([HAVE_DECL_FLOORL]) HAVE_DECL_FREXPL=1; AC_SUBST([HAVE_DECL_FREXPL]) HAVE_DECL_LDEXPL=1; AC_SUBST([HAVE_DECL_LDEXPL]) HAVE_DECL_LOGL=1; AC_SUBST([HAVE_DECL_LOGL]) HAVE_DECL_LOG10L=1; AC_SUBST([HAVE_DECL_LOG10L]) HAVE_DECL_LOG2=1; AC_SUBST([HAVE_DECL_LOG2]) HAVE_DECL_LOG2F=1; AC_SUBST([HAVE_DECL_LOG2F]) HAVE_DECL_LOG2L=1; AC_SUBST([HAVE_DECL_LOG2L]) HAVE_DECL_LOGB=1; AC_SUBST([HAVE_DECL_LOGB]) HAVE_DECL_REMAINDER=1; AC_SUBST([HAVE_DECL_REMAINDER]) HAVE_DECL_REMAINDERL=1; AC_SUBST([HAVE_DECL_REMAINDERL]) HAVE_DECL_RINTF=1; AC_SUBST([HAVE_DECL_RINTF]) HAVE_DECL_ROUND=1; AC_SUBST([HAVE_DECL_ROUND]) HAVE_DECL_ROUNDF=1; AC_SUBST([HAVE_DECL_ROUNDF]) HAVE_DECL_ROUNDL=1; AC_SUBST([HAVE_DECL_ROUNDL]) HAVE_DECL_SINL=1; AC_SUBST([HAVE_DECL_SINL]) HAVE_DECL_SQRTL=1; AC_SUBST([HAVE_DECL_SQRTL]) HAVE_DECL_TANL=1; AC_SUBST([HAVE_DECL_TANL]) HAVE_DECL_TRUNC=1; AC_SUBST([HAVE_DECL_TRUNC]) HAVE_DECL_TRUNCF=1; AC_SUBST([HAVE_DECL_TRUNCF]) HAVE_DECL_TRUNCL=1; AC_SUBST([HAVE_DECL_TRUNCL]) REPLACE_CBRTF=0; AC_SUBST([REPLACE_CBRTF]) REPLACE_CBRTL=0; AC_SUBST([REPLACE_CBRTL]) REPLACE_CEIL=0; AC_SUBST([REPLACE_CEIL]) REPLACE_CEILF=0; AC_SUBST([REPLACE_CEILF]) REPLACE_CEILL=0; AC_SUBST([REPLACE_CEILL]) REPLACE_EXPM1=0; AC_SUBST([REPLACE_EXPM1]) REPLACE_EXPM1F=0; AC_SUBST([REPLACE_EXPM1F]) REPLACE_EXP2=0; AC_SUBST([REPLACE_EXP2]) REPLACE_EXP2L=0; AC_SUBST([REPLACE_EXP2L]) REPLACE_FABSL=0; AC_SUBST([REPLACE_FABSL]) REPLACE_FLOOR=0; AC_SUBST([REPLACE_FLOOR]) REPLACE_FLOORF=0; AC_SUBST([REPLACE_FLOORF]) REPLACE_FLOORL=0; AC_SUBST([REPLACE_FLOORL]) REPLACE_FMA=0; AC_SUBST([REPLACE_FMA]) REPLACE_FMAF=0; AC_SUBST([REPLACE_FMAF]) REPLACE_FMAL=0; AC_SUBST([REPLACE_FMAL]) REPLACE_FMOD=0; AC_SUBST([REPLACE_FMOD]) REPLACE_FMODF=0; AC_SUBST([REPLACE_FMODF]) REPLACE_FMODL=0; AC_SUBST([REPLACE_FMODL]) REPLACE_FREXPF=0; AC_SUBST([REPLACE_FREXPF]) REPLACE_FREXP=0; AC_SUBST([REPLACE_FREXP]) REPLACE_FREXPL=0; AC_SUBST([REPLACE_FREXPL]) REPLACE_HUGE_VAL=0; AC_SUBST([REPLACE_HUGE_VAL]) REPLACE_HYPOT=0; AC_SUBST([REPLACE_HYPOT]) REPLACE_HYPOTF=0; AC_SUBST([REPLACE_HYPOTF]) REPLACE_HYPOTL=0; AC_SUBST([REPLACE_HYPOTL]) REPLACE_ILOGB=0; AC_SUBST([REPLACE_ILOGB]) REPLACE_ILOGBF=0; AC_SUBST([REPLACE_ILOGBF]) REPLACE_ISFINITE=0; AC_SUBST([REPLACE_ISFINITE]) REPLACE_ISINF=0; AC_SUBST([REPLACE_ISINF]) REPLACE_ISNAN=0; AC_SUBST([REPLACE_ISNAN]) REPLACE_LDEXPL=0; AC_SUBST([REPLACE_LDEXPL]) REPLACE_LOG=0; AC_SUBST([REPLACE_LOG]) REPLACE_LOGF=0; AC_SUBST([REPLACE_LOGF]) REPLACE_LOGL=0; AC_SUBST([REPLACE_LOGL]) REPLACE_LOG10=0; AC_SUBST([REPLACE_LOG10]) REPLACE_LOG10F=0; AC_SUBST([REPLACE_LOG10F]) REPLACE_LOG10L=0; AC_SUBST([REPLACE_LOG10L]) REPLACE_LOG1P=0; AC_SUBST([REPLACE_LOG1P]) REPLACE_LOG1PF=0; AC_SUBST([REPLACE_LOG1PF]) REPLACE_LOG1PL=0; AC_SUBST([REPLACE_LOG1PL]) REPLACE_LOG2=0; AC_SUBST([REPLACE_LOG2]) REPLACE_LOG2F=0; AC_SUBST([REPLACE_LOG2F]) REPLACE_LOG2L=0; AC_SUBST([REPLACE_LOG2L]) REPLACE_LOGB=0; AC_SUBST([REPLACE_LOGB]) REPLACE_LOGBF=0; AC_SUBST([REPLACE_LOGBF]) REPLACE_LOGBL=0; AC_SUBST([REPLACE_LOGBL]) REPLACE_MODF=0; AC_SUBST([REPLACE_MODF]) REPLACE_MODFF=0; AC_SUBST([REPLACE_MODFF]) REPLACE_MODFL=0; AC_SUBST([REPLACE_MODFL]) REPLACE_NAN=0; AC_SUBST([REPLACE_NAN]) REPLACE_REMAINDER=0; AC_SUBST([REPLACE_REMAINDER]) REPLACE_REMAINDERF=0; AC_SUBST([REPLACE_REMAINDERF]) REPLACE_REMAINDERL=0; AC_SUBST([REPLACE_REMAINDERL]) REPLACE_ROUND=0; AC_SUBST([REPLACE_ROUND]) REPLACE_ROUNDF=0; AC_SUBST([REPLACE_ROUNDF]) REPLACE_ROUNDL=0; AC_SUBST([REPLACE_ROUNDL]) REPLACE_SIGNBIT=0; AC_SUBST([REPLACE_SIGNBIT]) REPLACE_SIGNBIT_USING_GCC=0; AC_SUBST([REPLACE_SIGNBIT_USING_GCC]) REPLACE_SQRTL=0; AC_SUBST([REPLACE_SQRTL]) REPLACE_TRUNC=0; AC_SUBST([REPLACE_TRUNC]) REPLACE_TRUNCF=0; AC_SUBST([REPLACE_TRUNCF]) REPLACE_TRUNCL=0; AC_SUBST([REPLACE_TRUNCL]) ]) # gl_LONG_DOUBLE_VS_DOUBLE # determines whether 'long double' and 'double' have the same representation. # Sets variable HAVE_SAME_LONG_DOUBLE_AS_DOUBLE to 0 or 1, and defines # HAVE_SAME_LONG_DOUBLE_AS_DOUBLE accordingly. # The currently known platforms where this is the case are: # Linux/HPPA, Minix 3.1.8, AIX 5, AIX 6 and 7 with xlc, MSVC 9. AC_DEFUN([gl_LONG_DOUBLE_VS_DOUBLE], [ AC_CACHE_CHECK([whether long double and double are the same], [gl_cv_long_double_equals_double], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include ]], [[typedef int check[sizeof (long double) == sizeof (double) && LDBL_MANT_DIG == DBL_MANT_DIG && LDBL_MAX_EXP == DBL_MAX_EXP && LDBL_MIN_EXP == DBL_MIN_EXP ? 1 : -1]; ]])], [gl_cv_long_double_equals_double=yes], [gl_cv_long_double_equals_double=no]) ]) if test $gl_cv_long_double_equals_double = yes; then AC_DEFINE([HAVE_SAME_LONG_DOUBLE_AS_DOUBLE], [1], [Define to 1 if 'long double' and 'double' have the same representation.]) HAVE_SAME_LONG_DOUBLE_AS_DOUBLE=1 else HAVE_SAME_LONG_DOUBLE_AS_DOUBLE=0 fi AC_SUBST([HAVE_SAME_LONG_DOUBLE_AS_DOUBLE]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/malloca.m40000644000175000017500000000110113004436755016015 00000000000000# malloca.m4 serial 1 dnl Copyright (C) 2003-2004, 2006-2007, 2009-2016 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_MALLOCA], [ dnl Use the autoconf tests for alloca(), but not the AC_SUBSTed variables dnl @ALLOCA@ and @LTALLOCA@. dnl gl_FUNC_ALLOCA dnl Already brought in by the module dependencies. AC_REQUIRE([gl_EEMALLOC]) AC_REQUIRE([AC_TYPE_LONG_LONG_INT]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/malloc.m40000644000175000017500000000642313004436755015670 00000000000000# malloc.m4 serial 15 dnl Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. m4_version_prereq([2.70], [] ,[ # This is adapted with modifications from upstream Autoconf here: # http://git.savannah.gnu.org/cgit/autoconf.git/commit/?id=04be2b7a29d65d9a08e64e8e56e594c91749598c AC_DEFUN([_AC_FUNC_MALLOC_IF], [ AC_REQUIRE([AC_HEADER_STDC])dnl AC_REQUIRE([AC_CANONICAL_HOST])dnl for cross-compiles AC_CHECK_HEADERS([stdlib.h]) AC_CACHE_CHECK([for GNU libc compatible malloc], [ac_cv_func_malloc_0_nonnull], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#if defined STDC_HEADERS || defined HAVE_STDLIB_H # include #else char *malloc (); #endif ]], [[char *p = malloc (0); int result = !p; free (p); return result;]]) ], [ac_cv_func_malloc_0_nonnull=yes], [ac_cv_func_malloc_0_nonnull=no], [case "$host_os" in # Guess yes on platforms where we know the result. *-gnu* | freebsd* | netbsd* | openbsd* \ | hpux* | solaris* | cygwin* | mingw*) ac_cv_func_malloc_0_nonnull=yes ;; # If we don't know, assume the worst. *) ac_cv_func_malloc_0_nonnull=no ;; esac ]) ]) AS_IF([test $ac_cv_func_malloc_0_nonnull = yes], [$1], [$2]) ])# _AC_FUNC_MALLOC_IF ]) # gl_FUNC_MALLOC_GNU # ------------------ # Test whether 'malloc (0)' is handled like in GNU libc, and replace malloc if # it is not. AC_DEFUN([gl_FUNC_MALLOC_GNU], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) dnl _AC_FUNC_MALLOC_IF is defined in Autoconf. _AC_FUNC_MALLOC_IF( [AC_DEFINE([HAVE_MALLOC_GNU], [1], [Define to 1 if your system has a GNU libc compatible 'malloc' function, and to 0 otherwise.])], [AC_DEFINE([HAVE_MALLOC_GNU], [0]) REPLACE_MALLOC=1 ]) ]) # gl_FUNC_MALLOC_POSIX # -------------------- # Test whether 'malloc' is POSIX compliant (sets errno to ENOMEM when it # fails), and replace malloc if it is not. AC_DEFUN([gl_FUNC_MALLOC_POSIX], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) AC_REQUIRE([gl_CHECK_MALLOC_POSIX]) if test $gl_cv_func_malloc_posix = yes; then AC_DEFINE([HAVE_MALLOC_POSIX], [1], [Define if the 'malloc' function is POSIX compliant.]) else REPLACE_MALLOC=1 fi ]) # Test whether malloc, realloc, calloc are POSIX compliant, # Set gl_cv_func_malloc_posix to yes or no accordingly. AC_DEFUN([gl_CHECK_MALLOC_POSIX], [ AC_CACHE_CHECK([whether malloc, realloc, calloc are POSIX compliant], [gl_cv_func_malloc_posix], [ dnl It is too dangerous to try to allocate a large amount of memory: dnl some systems go to their knees when you do that. So assume that dnl all Unix implementations of the function are POSIX compliant. 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the Free Software Foundation gives # unlimited permission to copy and/or distribute it, with or without # modifications, as long as this notice is preserved. # @configure_input@ # serial 4179 ltversion.m4 # This file is part of GNU Libtool m4_define([LT_PACKAGE_VERSION], [2.4.6]) m4_define([LT_PACKAGE_REVISION], [2.4.6]) AC_DEFUN([LTVERSION_VERSION], [macro_version='2.4.6' macro_revision='2.4.6' _LT_DECL(, macro_version, 0, [Which release of libtool.m4 was used?]) _LT_DECL(, macro_revision, 0) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/ltsugar.m40000644000175000017500000001044013004436745016073 00000000000000# ltsugar.m4 -- libtool m4 base layer. -*-Autoconf-*- # # Copyright (C) 2004-2005, 2007-2008, 2011-2015 Free Software # Foundation, Inc. # Written by Gary V. Vaughan, 2004 # # This file is free software; the Free Software Foundation gives # unlimited permission to copy and/or distribute it, with or without # modifications, as long as this notice is preserved. # serial 6 ltsugar.m4 # This is to help aclocal find these macros, as it can't see m4_define. AC_DEFUN([LTSUGAR_VERSION], [m4_if([0.1])]) # lt_join(SEP, ARG1, [ARG2...]) # ----------------------------- # Produce ARG1SEPARG2...SEPARGn, omitting [] arguments and their # associated separator. # Needed until we can rely on m4_join from Autoconf 2.62, since all earlier # versions in m4sugar had bugs. m4_define([lt_join], [m4_if([$#], [1], [], [$#], [2], [[$2]], [m4_if([$2], [], [], [[$2]_])$0([$1], m4_shift(m4_shift($@)))])]) m4_define([_lt_join], [m4_if([$#$2], [2], [], [m4_if([$2], [], [], [[$1$2]])$0([$1], m4_shift(m4_shift($@)))])]) # lt_car(LIST) # lt_cdr(LIST) # ------------ # Manipulate m4 lists. # These macros are necessary as long as will still need to support # Autoconf-2.59, which quotes differently. m4_define([lt_car], [[$1]]) m4_define([lt_cdr], [m4_if([$#], 0, [m4_fatal([$0: cannot be called without arguments])], [$#], 1, [], [m4_dquote(m4_shift($@))])]) m4_define([lt_unquote], $1) # lt_append(MACRO-NAME, STRING, [SEPARATOR]) # ------------------------------------------ # Redefine MACRO-NAME to hold its former content plus 'SEPARATOR''STRING'. # Note that neither SEPARATOR nor STRING are expanded; they are appended # to MACRO-NAME as is (leaving the expansion for when MACRO-NAME is invoked). # No SEPARATOR is output if MACRO-NAME was previously undefined (different # than defined and empty). # # This macro is needed until we can rely on Autoconf 2.62, since earlier # versions of m4sugar mistakenly expanded SEPARATOR but not STRING. m4_define([lt_append], [m4_define([$1], m4_ifdef([$1], [m4_defn([$1])[$3]])[$2])]) # lt_combine(SEP, PREFIX-LIST, INFIX, SUFFIX1, [SUFFIX2...]) # ---------------------------------------------------------- # Produce a SEP delimited list of all paired combinations of elements of # PREFIX-LIST with SUFFIX1 through SUFFIXn. Each element of the list # has the form PREFIXmINFIXSUFFIXn. # Needed until we can rely on m4_combine added in Autoconf 2.62. m4_define([lt_combine], [m4_if(m4_eval([$# > 3]), [1], [m4_pushdef([_Lt_sep], [m4_define([_Lt_sep], m4_defn([lt_car]))])]]dnl [[m4_foreach([_Lt_prefix], [$2], [m4_foreach([_Lt_suffix], ]m4_dquote(m4_dquote(m4_shift(m4_shift(m4_shift($@)))))[, [_Lt_sep([$1])[]m4_defn([_Lt_prefix])[$3]m4_defn([_Lt_suffix])])])])]) # lt_if_append_uniq(MACRO-NAME, VARNAME, [SEPARATOR], [UNIQ], [NOT-UNIQ]) # ----------------------------------------------------------------------- # Iff MACRO-NAME does not yet contain VARNAME, then append it (delimited # by SEPARATOR if supplied) and expand UNIQ, else NOT-UNIQ. m4_define([lt_if_append_uniq], [m4_ifdef([$1], [m4_if(m4_index([$3]m4_defn([$1])[$3], [$3$2$3]), [-1], [lt_append([$1], [$2], [$3])$4], [$5])], [lt_append([$1], [$2], [$3])$4])]) # lt_dict_add(DICT, KEY, VALUE) # ----------------------------- m4_define([lt_dict_add], [m4_define([$1($2)], [$3])]) # lt_dict_add_subkey(DICT, KEY, SUBKEY, VALUE) # -------------------------------------------- m4_define([lt_dict_add_subkey], [m4_define([$1($2:$3)], [$4])]) # lt_dict_fetch(DICT, KEY, [SUBKEY]) # ---------------------------------- m4_define([lt_dict_fetch], [m4_ifval([$3], m4_ifdef([$1($2:$3)], [m4_defn([$1($2:$3)])]), m4_ifdef([$1($2)], [m4_defn([$1($2)])]))]) # lt_if_dict_fetch(DICT, KEY, [SUBKEY], VALUE, IF-TRUE, [IF-FALSE]) # ----------------------------------------------------------------- m4_define([lt_if_dict_fetch], [m4_if(lt_dict_fetch([$1], [$2], [$3]), [$4], [$5], [$6])]) # lt_dict_filter(DICT, [SUBKEY], VALUE, [SEPARATOR], KEY, [...]) # -------------------------------------------------------------- m4_define([lt_dict_filter], [m4_if([$5], [], [], [lt_join(m4_quote(m4_default([$4], [[, ]])), lt_unquote(m4_split(m4_normalize(m4_foreach(_Lt_key, lt_car([m4_shiftn(4, $@)]), [lt_if_dict_fetch([$1], _Lt_key, [$2], [$3], [_Lt_key ])])))))])[]dnl ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/ltoptions.m40000644000175000017500000003426213004436745016455 00000000000000# Helper functions for option handling. -*- Autoconf -*- # # Copyright (C) 2004-2005, 2007-2009, 2011-2015 Free Software # Foundation, Inc. # Written by Gary V. Vaughan, 2004 # # This file is free software; the Free Software Foundation gives # unlimited permission to copy and/or distribute it, with or without # modifications, as long as this notice is preserved. # serial 8 ltoptions.m4 # This is to help aclocal find these macros, as it can't see m4_define. AC_DEFUN([LTOPTIONS_VERSION], [m4_if([1])]) # _LT_MANGLE_OPTION(MACRO-NAME, OPTION-NAME) # ------------------------------------------ m4_define([_LT_MANGLE_OPTION], [[_LT_OPTION_]m4_bpatsubst($1__$2, [[^a-zA-Z0-9_]], [_])]) # _LT_SET_OPTION(MACRO-NAME, OPTION-NAME) # --------------------------------------- # Set option OPTION-NAME for macro MACRO-NAME, and if there is a # matching handler defined, dispatch to it. 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We use all the common list separators. lt_save_ifs=$IFS; IFS=$IFS$PATH_SEPARATOR, for pkg in $enableval; do IFS=$lt_save_ifs if test "X$pkg" = "X$p"; then enable_static=yes fi done IFS=$lt_save_ifs ;; esac], [enable_static=]_LT_ENABLE_STATIC_DEFAULT) _LT_DECL([build_old_libs], [enable_static], [0], [Whether or not to build static libraries]) ])# _LT_ENABLE_STATIC LT_OPTION_DEFINE([LT_INIT], [static], [_LT_ENABLE_STATIC([yes])]) LT_OPTION_DEFINE([LT_INIT], [disable-static], [_LT_ENABLE_STATIC([no])]) # Old names: AC_DEFUN([AC_ENABLE_STATIC], [_LT_SET_OPTION([LT_INIT], m4_if([$1], [no], [disable-])[static]) ]) AC_DEFUN([AC_DISABLE_STATIC], [_LT_SET_OPTION([LT_INIT], [disable-static]) ]) AU_DEFUN([AM_ENABLE_STATIC], [AC_ENABLE_STATIC($@)]) AU_DEFUN([AM_DISABLE_STATIC], [AC_DISABLE_STATIC($@)]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AM_ENABLE_STATIC], []) dnl AC_DEFUN([AM_DISABLE_STATIC], []) # _LT_ENABLE_FAST_INSTALL([DEFAULT]) # ---------------------------------- # implement the --enable-fast-install flag, and support the 'fast-install' # and 'disable-fast-install' LT_INIT options. # DEFAULT is either 'yes' or 'no'. If omitted, it defaults to 'yes'. m4_define([_LT_ENABLE_FAST_INSTALL], [m4_define([_LT_ENABLE_FAST_INSTALL_DEFAULT], [m4_if($1, no, no, yes)])dnl AC_ARG_ENABLE([fast-install], [AS_HELP_STRING([--enable-fast-install@<:@=PKGS@:>@], [optimize for fast installation @<:@default=]_LT_ENABLE_FAST_INSTALL_DEFAULT[@:>@])], [p=${PACKAGE-default} case $enableval in yes) enable_fast_install=yes ;; no) enable_fast_install=no ;; *) enable_fast_install=no # Look at the argument we got. We use all the common list separators. lt_save_ifs=$IFS; IFS=$IFS$PATH_SEPARATOR, for pkg in $enableval; do IFS=$lt_save_ifs if test "X$pkg" = "X$p"; then enable_fast_install=yes fi done IFS=$lt_save_ifs ;; esac], [enable_fast_install=]_LT_ENABLE_FAST_INSTALL_DEFAULT) _LT_DECL([fast_install], [enable_fast_install], [0], [Whether or not to optimize for fast installation])dnl ])# _LT_ENABLE_FAST_INSTALL LT_OPTION_DEFINE([LT_INIT], [fast-install], [_LT_ENABLE_FAST_INSTALL([yes])]) LT_OPTION_DEFINE([LT_INIT], [disable-fast-install], [_LT_ENABLE_FAST_INSTALL([no])]) # Old names: AU_DEFUN([AC_ENABLE_FAST_INSTALL], [_LT_SET_OPTION([LT_INIT], m4_if([$1], [no], [disable-])[fast-install]) AC_DIAGNOSE([obsolete], [$0: Remove this warning and the call to _LT_SET_OPTION when you put the 'fast-install' option into LT_INIT's first parameter.]) ]) AU_DEFUN([AC_DISABLE_FAST_INSTALL], [_LT_SET_OPTION([LT_INIT], [disable-fast-install]) AC_DIAGNOSE([obsolete], [$0: Remove this warning and the call to _LT_SET_OPTION when you put the 'disable-fast-install' option into LT_INIT's first parameter.]) ]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AC_ENABLE_FAST_INSTALL], []) dnl AC_DEFUN([AM_DISABLE_FAST_INSTALL], []) # _LT_WITH_AIX_SONAME([DEFAULT]) # ---------------------------------- # implement the --with-aix-soname flag, and support the `aix-soname=aix' # and `aix-soname=both' and `aix-soname=svr4' LT_INIT options. DEFAULT # is either `aix', `both' or `svr4'. If omitted, it defaults to `aix'. m4_define([_LT_WITH_AIX_SONAME], [m4_define([_LT_WITH_AIX_SONAME_DEFAULT], [m4_if($1, svr4, svr4, m4_if($1, both, both, aix))])dnl shared_archive_member_spec= case $host,$enable_shared in power*-*-aix[[5-9]]*,yes) AC_MSG_CHECKING([which variant of shared library versioning to provide]) AC_ARG_WITH([aix-soname], [AS_HELP_STRING([--with-aix-soname=aix|svr4|both], [shared library versioning (aka "SONAME") variant to provide on AIX, @<:@default=]_LT_WITH_AIX_SONAME_DEFAULT[@:>@.])], [case $withval in aix|svr4|both) ;; *) AC_MSG_ERROR([Unknown argument to --with-aix-soname]) ;; esac lt_cv_with_aix_soname=$with_aix_soname], [AC_CACHE_VAL([lt_cv_with_aix_soname], [lt_cv_with_aix_soname=]_LT_WITH_AIX_SONAME_DEFAULT) with_aix_soname=$lt_cv_with_aix_soname]) AC_MSG_RESULT([$with_aix_soname]) if test aix != "$with_aix_soname"; then # For the AIX way of multilib, we name the shared archive member # based on the bitwidth used, traditionally 'shr.o' or 'shr_64.o', # and 'shr.imp' or 'shr_64.imp', respectively, for the Import File. # Even when GNU compilers ignore OBJECT_MODE but need '-maix64' flag, # the AIX toolchain works better with OBJECT_MODE set (default 32). if test 64 = "${OBJECT_MODE-32}"; then shared_archive_member_spec=shr_64 else shared_archive_member_spec=shr fi fi ;; *) with_aix_soname=aix ;; esac _LT_DECL([], [shared_archive_member_spec], [0], [Shared archive member basename, for filename based shared library versioning on AIX])dnl ])# _LT_WITH_AIX_SONAME LT_OPTION_DEFINE([LT_INIT], [aix-soname=aix], [_LT_WITH_AIX_SONAME([aix])]) LT_OPTION_DEFINE([LT_INIT], [aix-soname=both], [_LT_WITH_AIX_SONAME([both])]) LT_OPTION_DEFINE([LT_INIT], [aix-soname=svr4], [_LT_WITH_AIX_SONAME([svr4])]) # _LT_WITH_PIC([MODE]) # -------------------- # implement the --with-pic flag, and support the 'pic-only' and 'no-pic' # LT_INIT options. # MODE is either 'yes' or 'no'. If omitted, it defaults to 'both'. m4_define([_LT_WITH_PIC], [AC_ARG_WITH([pic], [AS_HELP_STRING([--with-pic@<:@=PKGS@:>@], [try to use only PIC/non-PIC objects @<:@default=use both@:>@])], [lt_p=${PACKAGE-default} case $withval in yes|no) pic_mode=$withval ;; *) pic_mode=default # Look at the argument we got. We use all the common list separators. lt_save_ifs=$IFS; IFS=$IFS$PATH_SEPARATOR, for lt_pkg in $withval; do IFS=$lt_save_ifs if test "X$lt_pkg" = "X$lt_p"; then pic_mode=yes fi done IFS=$lt_save_ifs ;; esac], [pic_mode=m4_default([$1], [default])]) _LT_DECL([], [pic_mode], [0], [What type of objects to build])dnl ])# _LT_WITH_PIC LT_OPTION_DEFINE([LT_INIT], [pic-only], [_LT_WITH_PIC([yes])]) LT_OPTION_DEFINE([LT_INIT], [no-pic], [_LT_WITH_PIC([no])]) # Old name: AU_DEFUN([AC_LIBTOOL_PICMODE], [_LT_SET_OPTION([LT_INIT], [pic-only]) AC_DIAGNOSE([obsolete], [$0: Remove this warning and the call to _LT_SET_OPTION when you put the 'pic-only' option into LT_INIT's first parameter.]) ]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AC_LIBTOOL_PICMODE], []) ## ----------------- ## ## LTDL_INIT Options ## ## ----------------- ## m4_define([_LTDL_MODE], []) LT_OPTION_DEFINE([LTDL_INIT], [nonrecursive], [m4_define([_LTDL_MODE], [nonrecursive])]) LT_OPTION_DEFINE([LTDL_INIT], [recursive], [m4_define([_LTDL_MODE], [recursive])]) LT_OPTION_DEFINE([LTDL_INIT], [subproject], [m4_define([_LTDL_MODE], [subproject])]) m4_define([_LTDL_TYPE], []) LT_OPTION_DEFINE([LTDL_INIT], [installable], [m4_define([_LTDL_TYPE], [installable])]) LT_OPTION_DEFINE([LTDL_INIT], [convenience], [m4_define([_LTDL_TYPE], [convenience])]) gnuastro-0.2.33-8a3b/bootstrapped/m4/lstat.m40000644000175000017500000000457713004436755015560 00000000000000# serial 27 # Copyright (C) 1997-2001, 2003-2016 Free Software Foundation, Inc. # # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. dnl From Jim Meyering. AC_DEFUN([gl_FUNC_LSTAT], [ AC_REQUIRE([gl_SYS_STAT_H_DEFAULTS]) dnl If lstat does not exist, the replacement does dnl "#define lstat stat", and lstat.c is a no-op. AC_CHECK_FUNCS_ONCE([lstat]) if test $ac_cv_func_lstat = yes; then AC_REQUIRE([gl_FUNC_LSTAT_FOLLOWS_SLASHED_SYMLINK]) case "$gl_cv_func_lstat_dereferences_slashed_symlink" in *no) REPLACE_LSTAT=1 ;; esac else HAVE_LSTAT=0 fi ]) # Prerequisites of lib/lstat.c. AC_DEFUN([gl_PREREQ_LSTAT], [:]) AC_DEFUN([gl_FUNC_LSTAT_FOLLOWS_SLASHED_SYMLINK], [ dnl We don't use AC_FUNC_LSTAT_FOLLOWS_SLASHED_SYMLINK any more, because it dnl is no longer maintained in Autoconf and because it invokes AC_LIBOBJ. AC_CACHE_CHECK([whether lstat correctly handles trailing slash], [gl_cv_func_lstat_dereferences_slashed_symlink], [rm -f conftest.sym conftest.file echo >conftest.file AC_RUN_IFELSE( [AC_LANG_PROGRAM( [AC_INCLUDES_DEFAULT], [[struct stat sbuf; if (symlink ("conftest.file", "conftest.sym") != 0) return 1; /* Linux will dereference the symlink and fail, as required by POSIX. That is better in the sense that it means we will not have to compile and use the lstat wrapper. */ return lstat ("conftest.sym/", &sbuf) == 0; ]])], [gl_cv_func_lstat_dereferences_slashed_symlink=yes], [gl_cv_func_lstat_dereferences_slashed_symlink=no], [case "$host_os" in *-gnu*) # Guess yes on glibc systems. gl_cv_func_lstat_dereferences_slashed_symlink="guessing yes" ;; *) # If we don't know, assume the worst. gl_cv_func_lstat_dereferences_slashed_symlink="guessing no" ;; esac ]) rm -f conftest.sym conftest.file ]) case "$gl_cv_func_lstat_dereferences_slashed_symlink" in *yes) AC_DEFINE_UNQUOTED([LSTAT_FOLLOWS_SLASHED_SYMLINK], [1], [Define to 1 if 'lstat' dereferences a symlink specified with a trailing slash.]) ;; esac ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/longlong.m40000644000175000017500000001120313004436755016230 00000000000000# longlong.m4 serial 17 dnl Copyright (C) 1999-2007, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Paul Eggert. # Define HAVE_LONG_LONG_INT if 'long long int' works. # This fixes a bug in Autoconf 2.61, and can be faster # than what's in Autoconf 2.62 through 2.68. # Note: If the type 'long long int' exists but is only 32 bits large # (as on some very old compilers), HAVE_LONG_LONG_INT will not be # defined. In this case you can treat 'long long int' like 'long int'. AC_DEFUN([AC_TYPE_LONG_LONG_INT], [ AC_REQUIRE([AC_TYPE_UNSIGNED_LONG_LONG_INT]) AC_CACHE_CHECK([for long long int], [ac_cv_type_long_long_int], [ac_cv_type_long_long_int=yes if test "x${ac_cv_prog_cc_c99-no}" = xno; then ac_cv_type_long_long_int=$ac_cv_type_unsigned_long_long_int if test $ac_cv_type_long_long_int = yes; then dnl Catch a bug in Tandem NonStop Kernel (OSS) cc -O circa 2004. dnl If cross compiling, assume the bug is not important, since dnl nobody cross compiles for this platform as far as we know. AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[@%:@include @%:@ifndef LLONG_MAX @%:@ define HALF \ (1LL << (sizeof (long long int) * CHAR_BIT - 2)) @%:@ define LLONG_MAX (HALF - 1 + HALF) @%:@endif]], [[long long int n = 1; int i; for (i = 0; ; i++) { long long int m = n << i; if (m >> i != n) return 1; if (LLONG_MAX / 2 < m) break; } return 0;]])], [], [ac_cv_type_long_long_int=no], [:]) fi fi]) if test $ac_cv_type_long_long_int = yes; then AC_DEFINE([HAVE_LONG_LONG_INT], [1], [Define to 1 if the system has the type 'long long int'.]) fi ]) # Define HAVE_UNSIGNED_LONG_LONG_INT if 'unsigned long long int' works. # This fixes a bug in Autoconf 2.61, and can be faster # than what's in Autoconf 2.62 through 2.68. # Note: If the type 'unsigned long long int' exists but is only 32 bits # large (as on some very old compilers), AC_TYPE_UNSIGNED_LONG_LONG_INT # will not be defined. In this case you can treat 'unsigned long long int' # like 'unsigned long int'. AC_DEFUN([AC_TYPE_UNSIGNED_LONG_LONG_INT], [ AC_CACHE_CHECK([for unsigned long long int], [ac_cv_type_unsigned_long_long_int], [ac_cv_type_unsigned_long_long_int=yes if test "x${ac_cv_prog_cc_c99-no}" = xno; then AC_LINK_IFELSE( [_AC_TYPE_LONG_LONG_SNIPPET], [], [ac_cv_type_unsigned_long_long_int=no]) fi]) if test $ac_cv_type_unsigned_long_long_int = yes; then AC_DEFINE([HAVE_UNSIGNED_LONG_LONG_INT], [1], [Define to 1 if the system has the type 'unsigned long long int'.]) fi ]) # Expands to a C program that can be used to test for simultaneous support # of 'long long' and 'unsigned long long'. We don't want to say that # 'long long' is available if 'unsigned long long' is not, or vice versa, # because too many programs rely on the symmetry between signed and unsigned # integer types (excluding 'bool'). AC_DEFUN([_AC_TYPE_LONG_LONG_SNIPPET], [ AC_LANG_PROGRAM( [[/* For now, do not test the preprocessor; as of 2007 there are too many implementations with broken preprocessors. Perhaps this can be revisited in 2012. In the meantime, code should not expect #if to work with literals wider than 32 bits. */ /* Test literals. */ long long int ll = 9223372036854775807ll; long long int nll = -9223372036854775807LL; unsigned long long int ull = 18446744073709551615ULL; /* Test constant expressions. */ typedef int a[((-9223372036854775807LL < 0 && 0 < 9223372036854775807ll) ? 1 : -1)]; typedef int b[(18446744073709551615ULL <= (unsigned long long int) -1 ? 1 : -1)]; int i = 63;]], [[/* Test availability of runtime routines for shift and division. */ long long int llmax = 9223372036854775807ll; unsigned long long int ullmax = 18446744073709551615ull; return ((ll << 63) | (ll >> 63) | (ll < i) | (ll > i) | (llmax / ll) | (llmax % ll) | (ull << 63) | (ull >> 63) | (ull << i) | (ull >> i) | (ullmax / ull) | (ullmax % ull));]]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/lock.m40000644000175000017500000000266713004436755015357 00000000000000# lock.m4 serial 13 (gettext-0.18.2) dnl Copyright (C) 2005-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. AC_DEFUN([gl_LOCK], [ AC_REQUIRE([gl_THREADLIB]) if test "$gl_threads_api" = posix; then # OSF/1 4.0 and Mac OS X 10.1 lack the pthread_rwlock_t type and the # pthread_rwlock_* functions. AC_CHECK_TYPE([pthread_rwlock_t], [AC_DEFINE([HAVE_PTHREAD_RWLOCK], [1], [Define if the POSIX multithreading library has read/write locks.])], [], [#include ]) # glibc defines PTHREAD_MUTEX_RECURSIVE as enum, not as a macro. AC_COMPILE_IFELSE([ AC_LANG_PROGRAM( [[#include ]], [[ #if __FreeBSD__ == 4 error "No, in FreeBSD 4.0 recursive mutexes actually don't work." #elif (defined __ENVIRONMENT_MAC_OS_X_VERSION_MIN_REQUIRED__ \ && __ENVIRONMENT_MAC_OS_X_VERSION_MIN_REQUIRED__ < 1070) error "No, in Mac OS X < 10.7 recursive mutexes actually don't work." #else int x = (int)PTHREAD_MUTEX_RECURSIVE; return !x; #endif ]])], [AC_DEFINE([HAVE_PTHREAD_MUTEX_RECURSIVE], [1], [Define if the defines PTHREAD_MUTEX_RECURSIVE.])]) fi gl_PREREQ_LOCK ]) # Prerequisites of lib/glthread/lock.c. AC_DEFUN([gl_PREREQ_LOCK], [:]) gnuastro-0.2.33-8a3b/bootstrapped/m4/localename.m40000644000175000017500000000113413004436755016513 00000000000000# localename.m4 serial 2 dnl Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_LOCALENAME], [ AC_REQUIRE([gt_LC_MESSAGES]) AC_REQUIRE([gt_INTL_MACOSX]) AC_CHECK_FUNCS([setlocale uselocale]) dnl Solaris 12 provides getlocalename_l, while Illumos doesn't have dnl it nor the equivalent. if test $ac_cv_func_uselocale = yes; then AC_CHECK_FUNCS([getlocalename_l]) fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/localeconv.m40000644000175000017500000000114713004436755016544 00000000000000# localeconv.m4 serial 1 dnl Copyright (C) 2012-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_LOCALECONV], [ AC_REQUIRE([gl_LOCALE_H_DEFAULTS]) AC_REQUIRE([gl_LOCALE_H]) if test $REPLACE_STRUCT_LCONV = 1; then REPLACE_LOCALECONV=1 fi ]) # Prerequisites of lib/localeconv.c. AC_DEFUN([gl_PREREQ_LOCALECONV], [ AC_CHECK_MEMBERS([struct lconv.decimal_point], [], [], [[#include ]]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/locale_h.m40000644000175000017500000001040113004436755016156 00000000000000# locale_h.m4 serial 19 dnl Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_LOCALE_H], [ dnl Use AC_REQUIRE here, so that the default behavior below is expanded dnl once only, before all statements that occur in other macros. AC_REQUIRE([gl_LOCALE_H_DEFAULTS]) dnl Persuade glibc to define locale_t and the int_p_*, int_n_* dnl members of 'struct lconv'. AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) dnl If is replaced, then must also be replaced. AC_REQUIRE([gl_STDDEF_H]) dnl Solaris 11 2011-11 defines the int_p_*, int_n_* members of 'struct lconv' dnl only if _LCONV_C99 is defined. AC_REQUIRE([AC_CANONICAL_HOST]) case "$host_os" in solaris*) AC_DEFINE([_LCONV_C99], [1], [Define to 1 on Solaris.]) ;; esac AC_CACHE_CHECK([whether locale.h conforms to POSIX:2001], [gl_cv_header_locale_h_posix2001], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include int x = LC_MESSAGES; int y = sizeof (((struct lconv *) 0)->decimal_point);]], [[]])], [gl_cv_header_locale_h_posix2001=yes], [gl_cv_header_locale_h_posix2001=no])]) dnl Check for . AC_CHECK_HEADERS_ONCE([xlocale.h]) if test $ac_cv_header_xlocale_h = yes; then HAVE_XLOCALE_H=1 dnl Check whether use of locale_t requires inclusion of , dnl e.g. on Mac OS X 10.5. If does not define locale_t by dnl itself, we assume that will do so. AC_CACHE_CHECK([whether locale.h defines locale_t], [gl_cv_header_locale_has_locale_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include locale_t x;]], [[]])], [gl_cv_header_locale_has_locale_t=yes], [gl_cv_header_locale_has_locale_t=no]) ]) if test $gl_cv_header_locale_has_locale_t = yes; then gl_cv_header_locale_h_needs_xlocale_h=no else gl_cv_header_locale_h_needs_xlocale_h=yes fi else HAVE_XLOCALE_H=0 gl_cv_header_locale_h_needs_xlocale_h=no fi AC_SUBST([HAVE_XLOCALE_H]) dnl Check whether 'struct lconv' is complete. dnl Bionic libc's 'struct lconv' is just a dummy. dnl On OpenBSD 4.9, HP-UX 11, IRIX 6.5, OSF/1 5.1, Solaris 9, Cygwin 1.5.x, dnl mingw, MSVC 9, it lacks the int_p_* and int_n_* members. AC_CACHE_CHECK([whether struct lconv is properly defined], [gl_cv_sys_struct_lconv_ok], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include struct lconv l; int x = sizeof (l.decimal_point); int y = sizeof (l.int_p_cs_precedes);]], [[]])], [gl_cv_sys_struct_lconv_ok=yes], [gl_cv_sys_struct_lconv_ok=no]) ]) if test $gl_cv_sys_struct_lconv_ok = no; then REPLACE_STRUCT_LCONV=1 fi dnl is always overridden, because of GNULIB_POSIXCHECK. gl_NEXT_HEADERS([locale.h]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[#include /* Some systems provide declarations in a non-standard header. */ #if HAVE_XLOCALE_H # include #endif ]], [setlocale duplocale]) ]) AC_DEFUN([gl_LOCALE_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_LOCALE_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_LOCALE_H_DEFAULTS], [ GNULIB_LOCALECONV=0; AC_SUBST([GNULIB_LOCALECONV]) GNULIB_SETLOCALE=0; AC_SUBST([GNULIB_SETLOCALE]) GNULIB_DUPLOCALE=0; AC_SUBST([GNULIB_DUPLOCALE]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_DUPLOCALE=1; AC_SUBST([HAVE_DUPLOCALE]) REPLACE_LOCALECONV=0; AC_SUBST([REPLACE_LOCALECONV]) REPLACE_SETLOCALE=0; AC_SUBST([REPLACE_SETLOCALE]) REPLACE_DUPLOCALE=0; AC_SUBST([REPLACE_DUPLOCALE]) REPLACE_STRUCT_LCONV=0; AC_SUBST([REPLACE_STRUCT_LCONV]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/locale-zh.m40000644000175000017500000001222613004436755016275 00000000000000# locale-zh.m4 serial 12 dnl Copyright (C) 2003, 2005-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl Determine the name of a chinese locale with GB18030 encoding. AC_DEFUN([gt_LOCALE_ZH_CN], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([AM_LANGINFO_CODESET]) AC_CACHE_CHECK([for a transitional chinese locale], [gt_cv_locale_zh_CN], [ AC_LANG_CONFTEST([AC_LANG_SOURCE([ changequote(,)dnl #include #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { const char *p; /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; /* Check whether a typical GB18030 multibyte sequence is recognized as a single wide character. This excludes the GB2312 and GBK encodings. */ if (mblen ("\203\062\332\066", 5) != 4) return 1; return 0; } changequote([,])dnl ])]) if AC_TRY_EVAL([ac_link]) && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=Chinese_China.54936 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=Chinese_China.54936 else # None found. gt_cv_locale_zh_CN=none fi ;; solaris2.8) # On Solaris 8, the locales zh_CN.GB18030, zh_CN.GBK, zh.GBK are # broken. One witness is the test case in gl_MBRTOWC_SANITYCHECK. # Another witness is that "LC_ALL=zh_CN.GB18030 bash -c true" dumps core. gt_cv_locale_zh_CN=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the locale name without encoding suffix. if (LC_ALL=zh_CN LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN else # Test for the locale name with explicit encoding suffix. if (LC_ALL=zh_CN.GB18030 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN.GB18030 else # None found. gt_cv_locale_zh_CN=none fi fi ;; esac else # If there was a link error, due to mblen(), the system is so old that # it certainly doesn't have a chinese locale. gt_cv_locale_zh_CN=none fi rm -fr conftest* ]) LOCALE_ZH_CN=$gt_cv_locale_zh_CN AC_SUBST([LOCALE_ZH_CN]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/locale-tr.m40000644000175000017500000001211113004436755016272 00000000000000# locale-tr.m4 serial 10 dnl Copyright (C) 2003, 2005-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl Determine the name of a turkish locale with UTF-8 encoding. AC_DEFUN([gt_LOCALE_TR_UTF8], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([AM_LANGINFO_CODESET]) AC_CACHE_CHECK([for a turkish Unicode locale], [gt_cv_locale_tr_utf8], [ AC_LANG_CONFTEST([AC_LANG_SOURCE([ changequote(,)dnl #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. But BeOS does not implement the Turkish upper-/lowercase mappings. Therefore, let this program return 1 on BeOS. */ /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the tr_TR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in the abbreviation of the eighth month, the second character (should be U+011F: LATIN SMALL LETTER G WITH BREVE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1992 - 1900; t.tm_mon = 8 - 1; t.tm_mday = 19; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc4 || buf[2] != (char) 0x9f) return 1; /* Check whether the upper-/lowercase mappings are as expected for Turkish. */ if (towupper ('i') != 0x0130 || towlower (0x0130) != 'i' || towupper(0x0131) != 'I' || towlower ('I') != 0x0131) return 1; return 0; } changequote([,])dnl ])]) if AC_TRY_EVAL([ac_link]) && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=Turkish_Turkey.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_tr_utf8=Turkish_Turkey.65001 else # None found. gt_cv_locale_tr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=tr_TR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_tr_utf8=tr_TR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=tr_TR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_tr_utf8=tr_TR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=tr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_tr_utf8=tr.UTF-8 else # None found. gt_cv_locale_tr_utf8=none fi fi fi ;; esac else gt_cv_locale_tr_utf8=none fi rm -fr conftest* ]) LOCALE_TR_UTF8=$gt_cv_locale_tr_utf8 AC_SUBST([LOCALE_TR_UTF8]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/locale-ja.m40000644000175000017500000001260313004436755016245 00000000000000# locale-ja.m4 serial 12 dnl Copyright (C) 2003, 2005-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl Determine the name of a japanese locale with EUC-JP encoding. AC_DEFUN([gt_LOCALE_JA], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([AM_LANGINFO_CODESET]) AC_CACHE_CHECK([for a traditional japanese locale], [gt_cv_locale_ja], [ AC_LANG_CONFTEST([AC_LANG_SOURCE([ changequote(,)dnl #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { const char *p; /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether MB_CUR_MAX is > 1. This excludes the dysfunctional locales on Cygwin 1.5.x. */ if (MB_CUR_MAX == 1) return 1; /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; return 0; } changequote([,])dnl ])]) if AC_TRY_EVAL([ac_link]) && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Note that on native Windows, the Japanese locale is # Japanese_Japan.932, and CP932 is very different from EUC-JP, so we # cannot use it here. gt_cv_locale_ja=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the AIX locale name. if (LC_ALL=ja_JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP else # Test for the locale name with explicit encoding suffix. if (LC_ALL=ja_JP.EUC-JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC-JP else # Test for the HP-UX, OSF/1, NetBSD locale name. if (LC_ALL=ja_JP.eucJP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.eucJP else # Test for the IRIX, FreeBSD locale name. if (LC_ALL=ja_JP.EUC LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC else # Test for the Solaris 7 locale name. if (LC_ALL=ja LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja else # Special test for NetBSD 1.6. if test -f /usr/share/locale/ja_JP.eucJP/LC_CTYPE; then gt_cv_locale_ja=ja_JP.eucJP else # None found. gt_cv_locale_ja=none fi fi fi fi fi fi ;; esac fi rm -fr conftest* ]) LOCALE_JA=$gt_cv_locale_ja AC_SUBST([LOCALE_JA]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/locale-fr.m40000644000175000017500000002422513004436755016265 00000000000000# locale-fr.m4 serial 17 dnl Copyright (C) 2003, 2005-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl Determine the name of a french locale with traditional encoding. AC_DEFUN([gt_LOCALE_FR], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([AM_LANGINFO_CODESET]) AC_CACHE_CHECK([for a traditional french locale], [gt_cv_locale_fr], [ AC_LANG_CONFTEST([AC_LANG_SOURCE([ changequote(,)dnl #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is only one byte long. This excludes the UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 3 || buf[2] != 'v') return 1; #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } changequote([,])dnl ])]) if AC_TRY_EVAL([ac_link]) && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the native Windows locale name. if (LC_ALL=French_France.1252 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=French_France.1252 else # None found. gt_cv_locale_fr=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.ISO-8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO-8859-1 else # Test for the AIX, OSF/1, FreeBSD, NetBSD, OpenBSD locale name. if (LC_ALL=fr_FR.ISO8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO8859-1 else # Test for the HP-UX locale name. if (LC_ALL=fr_FR.iso88591 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.iso88591 else # Test for the Solaris 7 locale name. if (LC_ALL=fr LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr else # None found. gt_cv_locale_fr=none fi fi fi fi fi ;; esac fi rm -fr conftest* ]) LOCALE_FR=$gt_cv_locale_fr AC_SUBST([LOCALE_FR]) ]) dnl Determine the name of a french locale with UTF-8 encoding. AC_DEFUN([gt_LOCALE_FR_UTF8], [ AC_REQUIRE([AM_LANGINFO_CODESET]) AC_CACHE_CHECK([for a french Unicode locale], [gt_cv_locale_fr_utf8], [ AC_LANG_CONFTEST([AC_LANG_SOURCE([ changequote(,)dnl #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if !(defined __BEOS__ || defined __HAIKU__) /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } changequote([,])dnl ])]) if AC_TRY_EVAL([ac_link]) && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* ]) LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 AC_SUBST([LOCALE_FR_UTF8]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/localcharset.m40000644000175000017500000000112513004436755017057 00000000000000# localcharset.m4 serial 7 dnl Copyright (C) 2002, 2004, 2006, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_LOCALCHARSET], [ dnl Prerequisites of lib/localcharset.c. AC_REQUIRE([AM_LANGINFO_CODESET]) AC_REQUIRE([gl_FCNTL_O_FLAGS]) AC_CHECK_DECLS_ONCE([getc_unlocked]) dnl Prerequisites of the lib/Makefile.am snippet. AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([gl_GLIBC21]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/limits-h.m40000644000175000017500000000202113004436755016135 00000000000000dnl Check whether limits.h has needed features. dnl Copyright 2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Paul Eggert. AC_DEFUN_ONCE([gl_LIMITS_H], [ gl_CHECK_NEXT_HEADERS([limits.h]) AC_CACHE_CHECK([whether limits.h has ULLONG_WIDTH etc.], [gl_cv_header_limits_width], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#ifndef __STDC_WANT_IEC_60559_BFP_EXT__ #define __STDC_WANT_IEC_60559_BFP_EXT__ 1 #endif #include int ullw = ULLONG_WIDTH;]])], [gl_cv_header_limits_width=yes], [gl_cv_header_limits_width=no])]) if test "$gl_cv_header_limits_width" = yes; then LIMITS_H= else LIMITS_H=limits.h fi AC_SUBST([LIMITS_H]) AM_CONDITIONAL([GL_GENERATE_LIMITS_H], [test -n "$LIMITS_H"]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/libtool.m40000644000175000017500000112507313004436745016070 00000000000000# libtool.m4 - Configure libtool for the host system. -*-Autoconf-*- # # Copyright (C) 1996-2001, 2003-2015 Free Software Foundation, Inc. # Written by Gordon Matzigkeit, 1996 # # This file is free software; the Free Software Foundation gives # unlimited permission to copy and/or distribute it, with or without # modifications, as long as this notice is preserved. m4_define([_LT_COPYING], [dnl # Copyright (C) 2014 Free Software Foundation, Inc. # This is free software; see the source for copying conditions. There is NO # warranty; not even for MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. # GNU Libtool is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 2 of of the License, or # (at your option) any later version. # # As a special exception to the GNU General Public License, if you # distribute this file as part of a program or library that is built # using GNU Libtool, you may include this file under the same # distribution terms that you use for the rest of that program. # # GNU Libtool is distributed in the hope that it will be useful, but # WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see . ]) # serial 58 LT_INIT # LT_PREREQ(VERSION) # ------------------ # Complain and exit if this libtool version is less that VERSION. m4_defun([LT_PREREQ], [m4_if(m4_version_compare(m4_defn([LT_PACKAGE_VERSION]), [$1]), -1, [m4_default([$3], [m4_fatal([Libtool version $1 or higher is required], 63)])], [$2])]) # _LT_CHECK_BUILDDIR # ------------------ # Complain if the absolute build directory name contains unusual characters m4_defun([_LT_CHECK_BUILDDIR], [case `pwd` in *\ * | *\ *) AC_MSG_WARN([Libtool does not cope well with whitespace in `pwd`]) ;; esac ]) # LT_INIT([OPTIONS]) # ------------------ AC_DEFUN([LT_INIT], [AC_PREREQ([2.62])dnl We use AC_PATH_PROGS_FEATURE_CHECK AC_REQUIRE([AC_CONFIG_AUX_DIR_DEFAULT])dnl AC_BEFORE([$0], [LT_LANG])dnl AC_BEFORE([$0], [LT_OUTPUT])dnl AC_BEFORE([$0], [LTDL_INIT])dnl m4_require([_LT_CHECK_BUILDDIR])dnl dnl Autoconf doesn't catch unexpanded LT_ macros by default: m4_pattern_forbid([^_?LT_[A-Z_]+$])dnl m4_pattern_allow([^(_LT_EOF|LT_DLGLOBAL|LT_DLLAZY_OR_NOW|LT_MULTI_MODULE)$])dnl dnl aclocal doesn't pull ltoptions.m4, ltsugar.m4, or ltversion.m4 dnl unless we require an AC_DEFUNed macro: AC_REQUIRE([LTOPTIONS_VERSION])dnl AC_REQUIRE([LTSUGAR_VERSION])dnl AC_REQUIRE([LTVERSION_VERSION])dnl AC_REQUIRE([LTOBSOLETE_VERSION])dnl m4_require([_LT_PROG_LTMAIN])dnl _LT_SHELL_INIT([SHELL=${CONFIG_SHELL-/bin/sh}]) dnl Parse OPTIONS _LT_SET_OPTIONS([$0], [$1]) # This can be used to rebuild libtool when needed LIBTOOL_DEPS=$ltmain # Always use our own libtool. LIBTOOL='$(SHELL) $(top_builddir)/libtool' AC_SUBST(LIBTOOL)dnl _LT_SETUP # Only expand once: m4_define([LT_INIT]) ])# LT_INIT # Old names: AU_ALIAS([AC_PROG_LIBTOOL], [LT_INIT]) AU_ALIAS([AM_PROG_LIBTOOL], [LT_INIT]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AC_PROG_LIBTOOL], []) dnl AC_DEFUN([AM_PROG_LIBTOOL], []) # _LT_PREPARE_CC_BASENAME # ----------------------- m4_defun([_LT_PREPARE_CC_BASENAME], [ # Calculate cc_basename. Skip known compiler wrappers and cross-prefix. func_cc_basename () { for cc_temp in @S|@*""; do case $cc_temp in compile | *[[\\/]]compile | ccache | *[[\\/]]ccache ) ;; distcc | *[[\\/]]distcc | purify | *[[\\/]]purify ) ;; \-*) ;; *) break;; esac done func_cc_basename_result=`$ECHO "$cc_temp" | $SED "s%.*/%%; s%^$host_alias-%%"` } ])# _LT_PREPARE_CC_BASENAME # _LT_CC_BASENAME(CC) # ------------------- # It would be clearer to call AC_REQUIREs from _LT_PREPARE_CC_BASENAME, # but that macro is also expanded into generated libtool script, which # arranges for $SED and $ECHO to be set by different means. m4_defun([_LT_CC_BASENAME], [m4_require([_LT_PREPARE_CC_BASENAME])dnl AC_REQUIRE([_LT_DECL_SED])dnl AC_REQUIRE([_LT_PROG_ECHO_BACKSLASH])dnl func_cc_basename $1 cc_basename=$func_cc_basename_result ]) # _LT_FILEUTILS_DEFAULTS # ---------------------- # It is okay to use these file commands and assume they have been set # sensibly after 'm4_require([_LT_FILEUTILS_DEFAULTS])'. m4_defun([_LT_FILEUTILS_DEFAULTS], [: ${CP="cp -f"} : ${MV="mv -f"} : ${RM="rm -f"} ])# _LT_FILEUTILS_DEFAULTS # _LT_SETUP # --------- m4_defun([_LT_SETUP], [AC_REQUIRE([AC_CANONICAL_HOST])dnl AC_REQUIRE([AC_CANONICAL_BUILD])dnl AC_REQUIRE([_LT_PREPARE_SED_QUOTE_VARS])dnl AC_REQUIRE([_LT_PROG_ECHO_BACKSLASH])dnl _LT_DECL([], [PATH_SEPARATOR], [1], [The PATH separator for the build system])dnl dnl _LT_DECL([], [host_alias], [0], [The host system])dnl _LT_DECL([], [host], [0])dnl _LT_DECL([], [host_os], [0])dnl dnl _LT_DECL([], [build_alias], [0], [The build system])dnl _LT_DECL([], [build], [0])dnl _LT_DECL([], [build_os], [0])dnl dnl AC_REQUIRE([AC_PROG_CC])dnl AC_REQUIRE([LT_PATH_LD])dnl AC_REQUIRE([LT_PATH_NM])dnl dnl AC_REQUIRE([AC_PROG_LN_S])dnl test -z "$LN_S" && LN_S="ln -s" _LT_DECL([], [LN_S], [1], [Whether we need soft or hard links])dnl dnl AC_REQUIRE([LT_CMD_MAX_LEN])dnl _LT_DECL([objext], [ac_objext], [0], [Object file suffix (normally "o")])dnl _LT_DECL([], [exeext], [0], [Executable file suffix (normally "")])dnl dnl m4_require([_LT_FILEUTILS_DEFAULTS])dnl m4_require([_LT_CHECK_SHELL_FEATURES])dnl m4_require([_LT_PATH_CONVERSION_FUNCTIONS])dnl m4_require([_LT_CMD_RELOAD])dnl m4_require([_LT_CHECK_MAGIC_METHOD])dnl m4_require([_LT_CHECK_SHAREDLIB_FROM_LINKLIB])dnl m4_require([_LT_CMD_OLD_ARCHIVE])dnl m4_require([_LT_CMD_GLOBAL_SYMBOLS])dnl m4_require([_LT_WITH_SYSROOT])dnl m4_require([_LT_CMD_TRUNCATE])dnl _LT_CONFIG_LIBTOOL_INIT([ # See if we are running on zsh, and set the options that allow our # commands through without removal of \ escapes INIT. if test -n "\${ZSH_VERSION+set}"; then setopt NO_GLOB_SUBST fi ]) if test -n "${ZSH_VERSION+set}"; then setopt NO_GLOB_SUBST fi _LT_CHECK_OBJDIR m4_require([_LT_TAG_COMPILER])dnl case $host_os in aix3*) # AIX sometimes has problems with the GCC collect2 program. For some # reason, if we set the COLLECT_NAMES environment variable, the problems # vanish in a puff of smoke. if test set != "${COLLECT_NAMES+set}"; then COLLECT_NAMES= export COLLECT_NAMES fi ;; esac # Global variables: ofile=libtool can_build_shared=yes # All known linkers require a '.a' archive for static linking (except MSVC, # which needs '.lib'). libext=a with_gnu_ld=$lt_cv_prog_gnu_ld old_CC=$CC old_CFLAGS=$CFLAGS # Set sane defaults for various variables test -z "$CC" && CC=cc test -z "$LTCC" && LTCC=$CC test -z "$LTCFLAGS" && LTCFLAGS=$CFLAGS test -z "$LD" && LD=ld test -z "$ac_objext" && ac_objext=o _LT_CC_BASENAME([$compiler]) # Only perform the check for file, if the check method requires it test -z "$MAGIC_CMD" && MAGIC_CMD=file case $deplibs_check_method in file_magic*) if test "$file_magic_cmd" = '$MAGIC_CMD'; then _LT_PATH_MAGIC fi ;; esac # Use C for the default configuration in the libtool script LT_SUPPORTED_TAG([CC]) _LT_LANG_C_CONFIG _LT_LANG_DEFAULT_CONFIG _LT_CONFIG_COMMANDS ])# _LT_SETUP # _LT_PREPARE_SED_QUOTE_VARS # -------------------------- # Define a few sed substitution that help us do robust quoting. m4_defun([_LT_PREPARE_SED_QUOTE_VARS], [# Backslashify metacharacters that are still active within # double-quoted strings. sed_quote_subst='s/\([["`$\\]]\)/\\\1/g' # Same as above, but do not quote variable references. double_quote_subst='s/\([["`\\]]\)/\\\1/g' # Sed substitution to delay expansion of an escaped shell variable in a # double_quote_subst'ed string. delay_variable_subst='s/\\\\\\\\\\\$/\\\\\\$/g' # Sed substitution to delay expansion of an escaped single quote. delay_single_quote_subst='s/'\''/'\'\\\\\\\'\''/g' # Sed substitution to avoid accidental globbing in evaled expressions no_glob_subst='s/\*/\\\*/g' ]) # _LT_PROG_LTMAIN # --------------- # Note that this code is called both from 'configure', and 'config.status' # now that we use AC_CONFIG_COMMANDS to generate libtool. Notably, # 'config.status' has no value for ac_aux_dir unless we are using Automake, # so we pass a copy along to make sure it has a sensible value anyway. m4_defun([_LT_PROG_LTMAIN], [m4_ifdef([AC_REQUIRE_AUX_FILE], [AC_REQUIRE_AUX_FILE([ltmain.sh])])dnl _LT_CONFIG_LIBTOOL_INIT([ac_aux_dir='$ac_aux_dir']) ltmain=$ac_aux_dir/ltmain.sh ])# _LT_PROG_LTMAIN ## ------------------------------------- ## ## Accumulate code for creating libtool. ## ## ------------------------------------- ## # So that we can recreate a full libtool script including additional # tags, we accumulate the chunks of code to send to AC_CONFIG_COMMANDS # in macros and then make a single call at the end using the 'libtool' # label. # _LT_CONFIG_LIBTOOL_INIT([INIT-COMMANDS]) # ---------------------------------------- # Register INIT-COMMANDS to be passed to AC_CONFIG_COMMANDS later. m4_define([_LT_CONFIG_LIBTOOL_INIT], [m4_ifval([$1], [m4_append([_LT_OUTPUT_LIBTOOL_INIT], [$1 ])])]) # Initialize. m4_define([_LT_OUTPUT_LIBTOOL_INIT]) # _LT_CONFIG_LIBTOOL([COMMANDS]) # ------------------------------ # Register COMMANDS to be passed to AC_CONFIG_COMMANDS later. m4_define([_LT_CONFIG_LIBTOOL], [m4_ifval([$1], [m4_append([_LT_OUTPUT_LIBTOOL_COMMANDS], [$1 ])])]) # Initialize. m4_define([_LT_OUTPUT_LIBTOOL_COMMANDS]) # _LT_CONFIG_SAVE_COMMANDS([COMMANDS], [INIT_COMMANDS]) # ----------------------------------------------------- m4_defun([_LT_CONFIG_SAVE_COMMANDS], [_LT_CONFIG_LIBTOOL([$1]) _LT_CONFIG_LIBTOOL_INIT([$2]) ]) # _LT_FORMAT_COMMENT([COMMENT]) # ----------------------------- # Add leading comment marks to the start of each line, and a trailing # full-stop to the whole comment if one is not present already. m4_define([_LT_FORMAT_COMMENT], [m4_ifval([$1], [ m4_bpatsubst([m4_bpatsubst([$1], [^ *], [# ])], [['`$\]], [\\\&])]m4_bmatch([$1], [[!?.]$], [], [.]) )]) ## ------------------------ ## ## FIXME: Eliminate VARNAME ## ## ------------------------ ## # _LT_DECL([CONFIGNAME], VARNAME, VALUE, [DESCRIPTION], [IS-TAGGED?]) # ------------------------------------------------------------------- # CONFIGNAME is the name given to the value in the libtool script. # VARNAME is the (base) name used in the configure script. # VALUE may be 0, 1 or 2 for a computed quote escaped value based on # VARNAME. Any other value will be used directly. m4_define([_LT_DECL], [lt_if_append_uniq([lt_decl_varnames], [$2], [, ], [lt_dict_add_subkey([lt_decl_dict], [$2], [libtool_name], [m4_ifval([$1], [$1], [$2])]) lt_dict_add_subkey([lt_decl_dict], [$2], [value], [$3]) m4_ifval([$4], [lt_dict_add_subkey([lt_decl_dict], [$2], [description], [$4])]) lt_dict_add_subkey([lt_decl_dict], [$2], [tagged?], [m4_ifval([$5], [yes], [no])])]) ]) # _LT_TAGDECL([CONFIGNAME], VARNAME, VALUE, [DESCRIPTION]) # -------------------------------------------------------- m4_define([_LT_TAGDECL], [_LT_DECL([$1], [$2], [$3], [$4], [yes])]) # lt_decl_tag_varnames([SEPARATOR], [VARNAME1...]) # ------------------------------------------------ m4_define([lt_decl_tag_varnames], [_lt_decl_filter([tagged?], [yes], $@)]) # _lt_decl_filter(SUBKEY, VALUE, [SEPARATOR], [VARNAME1..]) # --------------------------------------------------------- m4_define([_lt_decl_filter], [m4_case([$#], [0], [m4_fatal([$0: too few arguments: $#])], [1], [m4_fatal([$0: too few arguments: $#: $1])], [2], [lt_dict_filter([lt_decl_dict], [$1], [$2], [], lt_decl_varnames)], [3], [lt_dict_filter([lt_decl_dict], [$1], [$2], [$3], lt_decl_varnames)], [lt_dict_filter([lt_decl_dict], $@)])[]dnl ]) # lt_decl_quote_varnames([SEPARATOR], [VARNAME1...]) # -------------------------------------------------- m4_define([lt_decl_quote_varnames], [_lt_decl_filter([value], [1], $@)]) # lt_decl_dquote_varnames([SEPARATOR], [VARNAME1...]) # --------------------------------------------------- m4_define([lt_decl_dquote_varnames], [_lt_decl_filter([value], [2], $@)]) # lt_decl_varnames_tagged([SEPARATOR], [VARNAME1...]) # --------------------------------------------------- m4_define([lt_decl_varnames_tagged], [m4_assert([$# <= 2])dnl _$0(m4_quote(m4_default([$1], [[, ]])), m4_ifval([$2], [[$2]], [m4_dquote(lt_decl_tag_varnames)]), m4_split(m4_normalize(m4_quote(_LT_TAGS)), [ ]))]) m4_define([_lt_decl_varnames_tagged], [m4_ifval([$3], [lt_combine([$1], [$2], [_], $3)])]) # lt_decl_all_varnames([SEPARATOR], [VARNAME1...]) # ------------------------------------------------ m4_define([lt_decl_all_varnames], [_$0(m4_quote(m4_default([$1], [[, ]])), m4_if([$2], [], m4_quote(lt_decl_varnames), m4_quote(m4_shift($@))))[]dnl ]) m4_define([_lt_decl_all_varnames], [lt_join($@, lt_decl_varnames_tagged([$1], lt_decl_tag_varnames([[, ]], m4_shift($@))))dnl ]) # _LT_CONFIG_STATUS_DECLARE([VARNAME]) # ------------------------------------ # Quote a variable value, and forward it to 'config.status' so that its # declaration there will have the same value as in 'configure'. VARNAME # must have a single quote delimited value for this to work. m4_define([_LT_CONFIG_STATUS_DECLARE], [$1='`$ECHO "$][$1" | $SED "$delay_single_quote_subst"`']) # _LT_CONFIG_STATUS_DECLARATIONS # ------------------------------ # We delimit libtool config variables with single quotes, so when # we write them to config.status, we have to be sure to quote all # embedded single quotes properly. In configure, this macro expands # each variable declared with _LT_DECL (and _LT_TAGDECL) into: # # ='`$ECHO "$" | $SED "$delay_single_quote_subst"`' m4_defun([_LT_CONFIG_STATUS_DECLARATIONS], [m4_foreach([_lt_var], m4_quote(lt_decl_all_varnames), [m4_n([_LT_CONFIG_STATUS_DECLARE(_lt_var)])])]) # _LT_LIBTOOL_TAGS # ---------------- # Output comment and list of tags supported by the script m4_defun([_LT_LIBTOOL_TAGS], [_LT_FORMAT_COMMENT([The names of the tagged configurations supported by this script])dnl available_tags='_LT_TAGS'dnl ]) # _LT_LIBTOOL_DECLARE(VARNAME, [TAG]) # ----------------------------------- # Extract the dictionary values for VARNAME (optionally with TAG) and # expand to a commented shell variable setting: # # # Some comment about what VAR is for. # visible_name=$lt_internal_name m4_define([_LT_LIBTOOL_DECLARE], [_LT_FORMAT_COMMENT(m4_quote(lt_dict_fetch([lt_decl_dict], [$1], [description])))[]dnl m4_pushdef([_libtool_name], m4_quote(lt_dict_fetch([lt_decl_dict], [$1], [libtool_name])))[]dnl m4_case(m4_quote(lt_dict_fetch([lt_decl_dict], [$1], [value])), [0], [_libtool_name=[$]$1], [1], [_libtool_name=$lt_[]$1], [2], [_libtool_name=$lt_[]$1], [_libtool_name=lt_dict_fetch([lt_decl_dict], [$1], [value])])[]dnl m4_ifval([$2], [_$2])[]m4_popdef([_libtool_name])[]dnl ]) # _LT_LIBTOOL_CONFIG_VARS # ----------------------- # Produce commented declarations of non-tagged libtool config variables # suitable for insertion in the LIBTOOL CONFIG section of the 'libtool' # script. Tagged libtool config variables (even for the LIBTOOL CONFIG # section) are produced by _LT_LIBTOOL_TAG_VARS. m4_defun([_LT_LIBTOOL_CONFIG_VARS], [m4_foreach([_lt_var], m4_quote(_lt_decl_filter([tagged?], [no], [], lt_decl_varnames)), [m4_n([_LT_LIBTOOL_DECLARE(_lt_var)])])]) # _LT_LIBTOOL_TAG_VARS(TAG) # ------------------------- m4_define([_LT_LIBTOOL_TAG_VARS], [m4_foreach([_lt_var], m4_quote(lt_decl_tag_varnames), [m4_n([_LT_LIBTOOL_DECLARE(_lt_var, [$1])])])]) # _LT_TAGVAR(VARNAME, [TAGNAME]) # ------------------------------ m4_define([_LT_TAGVAR], [m4_ifval([$2], [$1_$2], [$1])]) # _LT_CONFIG_COMMANDS # ------------------- # Send accumulated output to $CONFIG_STATUS. Thanks to the lists of # variables for single and double quote escaping we saved from calls # to _LT_DECL, we can put quote escaped variables declarations # into 'config.status', and then the shell code to quote escape them in # for loops in 'config.status'. Finally, any additional code accumulated # from calls to _LT_CONFIG_LIBTOOL_INIT is expanded. m4_defun([_LT_CONFIG_COMMANDS], [AC_PROVIDE_IFELSE([LT_OUTPUT], dnl If the libtool generation code has been placed in $CONFIG_LT, dnl instead of duplicating it all over again into config.status, dnl then we will have config.status run $CONFIG_LT later, so it dnl needs to know what name is stored there: [AC_CONFIG_COMMANDS([libtool], [$SHELL $CONFIG_LT || AS_EXIT(1)], [CONFIG_LT='$CONFIG_LT'])], dnl If the libtool generation code is destined for config.status, dnl expand the accumulated commands and init code now: [AC_CONFIG_COMMANDS([libtool], [_LT_OUTPUT_LIBTOOL_COMMANDS], [_LT_OUTPUT_LIBTOOL_COMMANDS_INIT])]) ])#_LT_CONFIG_COMMANDS # Initialize. m4_define([_LT_OUTPUT_LIBTOOL_COMMANDS_INIT], [ # The HP-UX ksh and POSIX shell print the target directory to stdout # if CDPATH is set. 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AC_DEFUN([LT_OUTPUT], [: ${CONFIG_LT=./config.lt} AC_MSG_NOTICE([creating $CONFIG_LT]) _LT_GENERATED_FILE_INIT(["$CONFIG_LT"], [# Run this file to recreate a libtool stub with the current configuration.]) cat >>"$CONFIG_LT" <<\_LTEOF lt_cl_silent=false exec AS_MESSAGE_LOG_FD>>config.log { echo AS_BOX([Running $as_me.]) } >&AS_MESSAGE_LOG_FD lt_cl_help="\ '$as_me' creates a local libtool stub from the current configuration, for use in further configure time tests before the real libtool is generated. Usage: $[0] [[OPTIONS]] -h, --help print this help, then exit -V, --version print version number, then exit -q, --quiet do not print progress messages -d, --debug don't remove temporary files Report bugs to ." lt_cl_version="\ m4_ifset([AC_PACKAGE_NAME], [AC_PACKAGE_NAME ])config.lt[]dnl m4_ifset([AC_PACKAGE_VERSION], [ AC_PACKAGE_VERSION]) configured by $[0], generated by m4_PACKAGE_STRING. Copyright (C) 2011 Free Software Foundation, Inc. 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We know it's impossible # because TPF is a cross-compiler, and we know how we open DSOs. lt_cv_dlopen=dlopen lt_cv_dlopen_libs= lt_cv_dlopen_self=no ;; *) AC_CHECK_FUNC([shl_load], [lt_cv_dlopen=shl_load], [AC_CHECK_LIB([dld], [shl_load], [lt_cv_dlopen=shl_load lt_cv_dlopen_libs=-ldld], [AC_CHECK_FUNC([dlopen], [lt_cv_dlopen=dlopen], [AC_CHECK_LIB([dl], [dlopen], [lt_cv_dlopen=dlopen lt_cv_dlopen_libs=-ldl], [AC_CHECK_LIB([svld], [dlopen], [lt_cv_dlopen=dlopen lt_cv_dlopen_libs=-lsvld], [AC_CHECK_LIB([dld], [dld_link], [lt_cv_dlopen=dld_link lt_cv_dlopen_libs=-ldld]) ]) ]) ]) ]) ]) ;; esac if test no = "$lt_cv_dlopen"; then enable_dlopen=no else enable_dlopen=yes fi case $lt_cv_dlopen in dlopen) save_CPPFLAGS=$CPPFLAGS test yes = "$ac_cv_header_dlfcn_h" && CPPFLAGS="$CPPFLAGS -DHAVE_DLFCN_H" save_LDFLAGS=$LDFLAGS wl=$lt_prog_compiler_wl eval LDFLAGS=\"\$LDFLAGS $export_dynamic_flag_spec\" save_LIBS=$LIBS LIBS="$lt_cv_dlopen_libs $LIBS" AC_CACHE_CHECK([whether a program can dlopen itself], lt_cv_dlopen_self, [dnl _LT_TRY_DLOPEN_SELF( lt_cv_dlopen_self=yes, lt_cv_dlopen_self=yes, lt_cv_dlopen_self=no, lt_cv_dlopen_self=cross) ]) if test yes = "$lt_cv_dlopen_self"; then wl=$lt_prog_compiler_wl eval LDFLAGS=\"\$LDFLAGS $lt_prog_compiler_static\" AC_CACHE_CHECK([whether a statically linked program can dlopen itself], lt_cv_dlopen_self_static, [dnl _LT_TRY_DLOPEN_SELF( lt_cv_dlopen_self_static=yes, lt_cv_dlopen_self_static=yes, lt_cv_dlopen_self_static=no, lt_cv_dlopen_self_static=cross) ]) fi CPPFLAGS=$save_CPPFLAGS LDFLAGS=$save_LDFLAGS LIBS=$save_LIBS ;; esac case $lt_cv_dlopen_self in yes|no) enable_dlopen_self=$lt_cv_dlopen_self ;; *) enable_dlopen_self=unknown ;; esac case $lt_cv_dlopen_self_static in yes|no) enable_dlopen_self_static=$lt_cv_dlopen_self_static ;; *) enable_dlopen_self_static=unknown ;; esac fi _LT_DECL([dlopen_support], [enable_dlopen], [0], [Whether dlopen is supported]) _LT_DECL([dlopen_self], [enable_dlopen_self], [0], [Whether dlopen of programs is supported]) _LT_DECL([dlopen_self_static], [enable_dlopen_self_static], [0], [Whether dlopen of statically linked programs is supported]) ])# LT_SYS_DLOPEN_SELF # Old name: AU_ALIAS([AC_LIBTOOL_DLOPEN_SELF], [LT_SYS_DLOPEN_SELF]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AC_LIBTOOL_DLOPEN_SELF], []) # _LT_COMPILER_C_O([TAGNAME]) # --------------------------- # Check to see if options -c and -o are simultaneously supported by compiler. # This macro does not hard code the compiler like AC_PROG_CC_C_O. m4_defun([_LT_COMPILER_C_O], [m4_require([_LT_DECL_SED])dnl m4_require([_LT_FILEUTILS_DEFAULTS])dnl m4_require([_LT_TAG_COMPILER])dnl AC_CACHE_CHECK([if $compiler supports -c -o file.$ac_objext], [_LT_TAGVAR(lt_cv_prog_compiler_c_o, $1)], [_LT_TAGVAR(lt_cv_prog_compiler_c_o, $1)=no $RM -r conftest 2>/dev/null mkdir conftest cd conftest mkdir out echo "$lt_simple_compile_test_code" > conftest.$ac_ext lt_compiler_flag="-o out/conftest2.$ac_objext" # Insert the option either (1) after the last *FLAGS variable, or # (2) before a word containing "conftest.", or (3) at the end. # Note that $ac_compile itself does not contain backslashes and begins # with a dollar sign (not a hyphen), so the echo should work correctly. lt_compile=`echo "$ac_compile" | $SED \ -e 's:.*FLAGS}\{0,1\} :&$lt_compiler_flag :; t' \ -e 's: [[^ ]]*conftest\.: $lt_compiler_flag&:; t' \ -e 's:$: $lt_compiler_flag:'` (eval echo "\"\$as_me:$LINENO: $lt_compile\"" >&AS_MESSAGE_LOG_FD) (eval "$lt_compile" 2>out/conftest.err) ac_status=$? cat out/conftest.err >&AS_MESSAGE_LOG_FD echo "$as_me:$LINENO: \$? = $ac_status" >&AS_MESSAGE_LOG_FD if (exit $ac_status) && test -s out/conftest2.$ac_objext then # The compiler can only warn and ignore the option if not recognized # So say no if there are warnings $ECHO "$_lt_compiler_boilerplate" | $SED '/^$/d' > out/conftest.exp $SED '/^$/d; /^ *+/d' out/conftest.err >out/conftest.er2 if test ! -s out/conftest.er2 || diff out/conftest.exp out/conftest.er2 >/dev/null; then _LT_TAGVAR(lt_cv_prog_compiler_c_o, $1)=yes fi fi chmod u+w . 2>&AS_MESSAGE_LOG_FD $RM conftest* # SGI C++ compiler will create directory out/ii_files/ for # template instantiation test -d out/ii_files && $RM out/ii_files/* && rmdir out/ii_files $RM out/* && rmdir out cd .. $RM -r conftest $RM conftest* ]) _LT_TAGDECL([compiler_c_o], [lt_cv_prog_compiler_c_o], [1], [Does compiler simultaneously support -c and -o options?]) ])# _LT_COMPILER_C_O # _LT_COMPILER_FILE_LOCKS([TAGNAME]) # ---------------------------------- # Check to see if we can do hard links to lock some files if needed m4_defun([_LT_COMPILER_FILE_LOCKS], [m4_require([_LT_ENABLE_LOCK])dnl m4_require([_LT_FILEUTILS_DEFAULTS])dnl _LT_COMPILER_C_O([$1]) hard_links=nottested if test no = "$_LT_TAGVAR(lt_cv_prog_compiler_c_o, $1)" && test no != "$need_locks"; then # do not overwrite the value of need_locks provided by the user AC_MSG_CHECKING([if we can lock with hard links]) hard_links=yes $RM conftest* ln conftest.a conftest.b 2>/dev/null && hard_links=no touch conftest.a ln conftest.a conftest.b 2>&5 || hard_links=no ln conftest.a conftest.b 2>/dev/null && hard_links=no AC_MSG_RESULT([$hard_links]) if test no = "$hard_links"; then AC_MSG_WARN(['$CC' does not support '-c -o', so 'make -j' may be unsafe]) need_locks=warn fi else need_locks=no fi _LT_DECL([], [need_locks], [1], [Must we lock files when doing compilation?]) ])# _LT_COMPILER_FILE_LOCKS # _LT_CHECK_OBJDIR # ---------------- m4_defun([_LT_CHECK_OBJDIR], [AC_CACHE_CHECK([for objdir], [lt_cv_objdir], [rm -f .libs 2>/dev/null mkdir .libs 2>/dev/null if test -d .libs; then lt_cv_objdir=.libs else # MS-DOS does not allow filenames that begin with a dot. lt_cv_objdir=_libs fi rmdir .libs 2>/dev/null]) objdir=$lt_cv_objdir _LT_DECL([], [objdir], [0], [The name of the directory that contains temporary libtool files])dnl m4_pattern_allow([LT_OBJDIR])dnl AC_DEFINE_UNQUOTED([LT_OBJDIR], "$lt_cv_objdir/", [Define to the sub-directory where libtool stores uninstalled libraries.]) ])# _LT_CHECK_OBJDIR # _LT_LINKER_HARDCODE_LIBPATH([TAGNAME]) # -------------------------------------- # Check hardcoding attributes. m4_defun([_LT_LINKER_HARDCODE_LIBPATH], [AC_MSG_CHECKING([how to hardcode library paths into programs]) _LT_TAGVAR(hardcode_action, $1)= if test -n "$_LT_TAGVAR(hardcode_libdir_flag_spec, $1)" || test -n "$_LT_TAGVAR(runpath_var, $1)" || test yes = "$_LT_TAGVAR(hardcode_automatic, $1)"; then # We can hardcode non-existent directories. if test no != "$_LT_TAGVAR(hardcode_direct, $1)" && # If the only mechanism to avoid hardcoding is shlibpath_var, we # have to relink, otherwise we might link with an installed library # when we should be linking with a yet-to-be-installed one ## test no != "$_LT_TAGVAR(hardcode_shlibpath_var, $1)" && test no != "$_LT_TAGVAR(hardcode_minus_L, $1)"; then # Linking always hardcodes the temporary library directory. _LT_TAGVAR(hardcode_action, $1)=relink else # We can link without hardcoding, and we can hardcode nonexisting dirs. _LT_TAGVAR(hardcode_action, $1)=immediate fi else # We cannot hardcode anything, or else we can only hardcode existing # directories. _LT_TAGVAR(hardcode_action, $1)=unsupported fi AC_MSG_RESULT([$_LT_TAGVAR(hardcode_action, $1)]) if test relink = "$_LT_TAGVAR(hardcode_action, $1)" || test yes = "$_LT_TAGVAR(inherit_rpath, $1)"; then # Fast installation is not supported enable_fast_install=no elif test yes = "$shlibpath_overrides_runpath" || test no = "$enable_shared"; then # Fast installation is not necessary enable_fast_install=needless fi _LT_TAGDECL([], [hardcode_action], [0], [How to hardcode a shared library path into an executable]) ])# _LT_LINKER_HARDCODE_LIBPATH # _LT_CMD_STRIPLIB # ---------------- m4_defun([_LT_CMD_STRIPLIB], [m4_require([_LT_DECL_EGREP]) striplib= old_striplib= AC_MSG_CHECKING([whether stripping libraries is possible]) if test -n "$STRIP" && $STRIP -V 2>&1 | $GREP "GNU strip" >/dev/null; then test -z "$old_striplib" && old_striplib="$STRIP --strip-debug" test -z "$striplib" && striplib="$STRIP --strip-unneeded" AC_MSG_RESULT([yes]) else # FIXME - insert some real tests, host_os isn't really good enough case $host_os in darwin*) if test -n "$STRIP"; then striplib="$STRIP -x" old_striplib="$STRIP -S" AC_MSG_RESULT([yes]) else AC_MSG_RESULT([no]) fi ;; *) AC_MSG_RESULT([no]) ;; esac fi _LT_DECL([], [old_striplib], [1], [Commands to strip libraries]) _LT_DECL([], [striplib], [1]) ])# _LT_CMD_STRIPLIB # _LT_PREPARE_MUNGE_PATH_LIST # --------------------------- # Make sure func_munge_path_list() is defined correctly. m4_defun([_LT_PREPARE_MUNGE_PATH_LIST], [[# func_munge_path_list VARIABLE PATH # ----------------------------------- # VARIABLE is name of variable containing _space_ separated list of # directories to be munged by the contents of PATH, which is string # having a format: # "DIR[:DIR]:" # string "DIR[ DIR]" will be prepended to VARIABLE # ":DIR[:DIR]" # string "DIR[ DIR]" will be appended to VARIABLE # "DIRP[:DIRP]::[DIRA:]DIRA" # string "DIRP[ DIRP]" will be prepended to VARIABLE and string # "DIRA[ DIRA]" will be appended to VARIABLE # "DIR[:DIR]" # VARIABLE will be replaced by "DIR[ DIR]" func_munge_path_list () { case x@S|@2 in x) ;; *:) eval @S|@1=\"`$ECHO @S|@2 | $SED 's/:/ /g'` \@S|@@S|@1\" ;; x:*) eval @S|@1=\"\@S|@@S|@1 `$ECHO @S|@2 | $SED 's/:/ /g'`\" ;; *::*) eval @S|@1=\"\@S|@@S|@1\ `$ECHO @S|@2 | $SED -e 's/.*:://' -e 's/:/ /g'`\" eval @S|@1=\"`$ECHO @S|@2 | $SED -e 's/::.*//' -e 's/:/ /g'`\ \@S|@@S|@1\" ;; *) eval @S|@1=\"`$ECHO @S|@2 | $SED 's/:/ /g'`\" ;; esac } ]])# _LT_PREPARE_PATH_LIST # _LT_SYS_DYNAMIC_LINKER([TAG]) # ----------------------------- # PORTME Fill in your ld.so characteristics m4_defun([_LT_SYS_DYNAMIC_LINKER], [AC_REQUIRE([AC_CANONICAL_HOST])dnl m4_require([_LT_DECL_EGREP])dnl m4_require([_LT_FILEUTILS_DEFAULTS])dnl m4_require([_LT_DECL_OBJDUMP])dnl m4_require([_LT_DECL_SED])dnl m4_require([_LT_CHECK_SHELL_FEATURES])dnl m4_require([_LT_PREPARE_MUNGE_PATH_LIST])dnl AC_MSG_CHECKING([dynamic linker characteristics]) m4_if([$1], [], [ if test yes = "$GCC"; then case $host_os in darwin*) lt_awk_arg='/^libraries:/,/LR/' ;; *) lt_awk_arg='/^libraries:/' ;; esac case $host_os in mingw* | cegcc*) lt_sed_strip_eq='s|=\([[A-Za-z]]:\)|\1|g' ;; *) lt_sed_strip_eq='s|=/|/|g' ;; esac lt_search_path_spec=`$CC -print-search-dirs | awk $lt_awk_arg | $SED -e "s/^libraries://" -e $lt_sed_strip_eq` case $lt_search_path_spec in *\;*) # if the path contains ";" then we assume it to be the separator # otherwise default to the standard path separator (i.e. ":") - it is # assumed that no part of a normal pathname contains ";" but that should # okay in the real world where ";" in dirpaths is itself problematic. lt_search_path_spec=`$ECHO "$lt_search_path_spec" | $SED 's/;/ /g'` ;; *) lt_search_path_spec=`$ECHO "$lt_search_path_spec" | $SED "s/$PATH_SEPARATOR/ /g"` ;; esac # Ok, now we have the path, separated by spaces, we can step through it # and add multilib dir if necessary... lt_tmp_lt_search_path_spec= lt_multi_os_dir=/`$CC $CPPFLAGS $CFLAGS $LDFLAGS -print-multi-os-directory 2>/dev/null` # ...but if some path component already ends with the multilib dir we assume # that all is fine and trust -print-search-dirs as is (GCC 4.2? or newer). case "$lt_multi_os_dir; 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then # AIX 5 supports IA64 library_names_spec='$libname$release$shared_ext$major $libname$release$shared_ext$versuffix $libname$shared_ext' shlibpath_var=LD_LIBRARY_PATH else # With GCC up to 2.95.x, collect2 would create an import file # for dependence libraries. 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Also, we use the # versioned .so libs for executables only if there is the -brtl # linker flag in LDFLAGS as well, or --with-aix-soname=svr4 only. # To allow for filename-based versioning support, we need to create # libNAME.so.V as an archive file, containing: # *) an Import File, referring to the versioned filename of the # archive as well as the shared archive member, telling the # bitwidth (32 or 64) of that shared object, and providing the # list of exported symbols of that shared object, eventually # decorated with the 'weak' keyword # *) the shared object with the F_LOADONLY flag set, to really avoid # it being seen by the linker. # At run time we better use the real file rather than another symlink, # but for link time we create the symlink libNAME.so -> libNAME.so.V case $with_aix_soname,$aix_use_runtimelinking in # AIX (on Power*) has no versioning support, so currently we cannot hardcode correct # soname into executable. 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do :; done~func_stripname "" ".so" "$n"~test "$func_stripname_result" = "$n" || func_append rmfiles " $odir/$func_stripname_result.$libext"' # We do not specify a path in Import Files, so LIBPATH fires. shlibpath_overrides_runpath=yes ;; *,no) # both, prefer aix dynamic_linker="AIX lib.a[(]lib.so.V[)], lib.so.V[(]$shared_archive_member_spec.o[)]" library_names_spec='$libname$release.a $libname.a' soname_spec='$libname$release$shared_ext$major' # unpreferred sharedlib libNAME.so.V and symlink libNAME.so need extra handling postinstall_cmds='test -z "$dlname" || $install_shared_prog $dir/$dlname $destdir/$dlname~test -z "$tstripme" || test -z "$striplib" || $striplib $destdir/$dlname~test -n "$linkname" || linkname=$realname~func_stripname "" ".a" "$linkname"~(cd "$destdir" && $LN_S -f $dlname $func_stripname_result.so)' postuninstall_cmds='test -z "$dlname" || func_append rmfiles " $odir/$dlname"~for n in $old_library $library_names; do :; done~func_stripname "" ".a" "$n"~func_append rmfiles " $odir/$func_stripname_result.so"' ;; esac shlibpath_var=LIBPATH fi ;; amigaos*) case $host_cpu in powerpc) # Since July 2007 AmigaOS4 officially supports .so libraries. # When compiling the executable, add -use-dynld -Lsobjs: to the compileline. library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' ;; m68k) library_names_spec='$libname.ixlibrary $libname.a' # Create ${libname}_ixlibrary.a entries in /sys/libs. finish_eval='for lib in `ls $libdir/*.ixlibrary 2>/dev/null`; do libname=`func_echo_all "$lib" | $SED '\''s%^.*/\([[^/]]*\)\.ixlibrary$%\1%'\''`; $RM /sys/libs/${libname}_ixlibrary.a; $show "cd /sys/libs && $LN_S $lib ${libname}_ixlibrary.a"; cd /sys/libs && $LN_S $lib ${libname}_ixlibrary.a || exit 1; done' ;; esac ;; beos*) library_names_spec='$libname$shared_ext' dynamic_linker="$host_os ld.so" shlibpath_var=LIBRARY_PATH ;; bsdi[[45]]*) version_type=linux # correct to gnu/linux during the next big refactor need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' finish_cmds='PATH="\$PATH:/sbin" ldconfig $libdir' shlibpath_var=LD_LIBRARY_PATH sys_lib_search_path_spec="/shlib /usr/lib /usr/X11/lib /usr/contrib/lib /lib /usr/local/lib" sys_lib_dlsearch_path_spec="/shlib /usr/lib /usr/local/lib" # the default ld.so.conf also contains /usr/contrib/lib and # /usr/X11R6/lib (/usr/X11 is a link to /usr/X11R6), but let us allow # libtool to hard-code these into programs ;; cygwin* | mingw* | pw32* | cegcc*) version_type=windows shrext_cmds=.dll need_version=no need_lib_prefix=no case $GCC,$cc_basename in yes,*) # gcc library_names_spec='$libname.dll.a' # DLL is installed to $(libdir)/../bin by postinstall_cmds postinstall_cmds='base_file=`basename \$file`~ dlpath=`$SHELL 2>&1 -c '\''. $dir/'\''\$base_file'\''i; echo \$dlname'\''`~ dldir=$destdir/`dirname \$dlpath`~ test -d \$dldir || mkdir -p \$dldir~ $install_prog $dir/$dlname \$dldir/$dlname~ chmod a+x \$dldir/$dlname~ if test -n '\''$stripme'\'' && test -n '\''$striplib'\''; then eval '\''$striplib \$dldir/$dlname'\'' || exit \$?; fi' postuninstall_cmds='dldll=`$SHELL 2>&1 -c '\''. $file; echo \$dlname'\''`~ dlpath=$dir/\$dldll~ $RM \$dlpath' shlibpath_overrides_runpath=yes case $host_os in cygwin*) # Cygwin DLLs use 'cyg' prefix rather than 'lib' soname_spec='`echo $libname | sed -e 's/^lib/cyg/'``echo $release | $SED -e 's/[[.]]/-/g'`$versuffix$shared_ext' m4_if([$1], [],[ sys_lib_search_path_spec="$sys_lib_search_path_spec /usr/lib/w32api"]) ;; 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esac ;; haiku*) version_type=linux # correct to gnu/linux during the next big refactor need_lib_prefix=no need_version=no dynamic_linker="$host_os runtime_loader" library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' shlibpath_var=LIBRARY_PATH shlibpath_overrides_runpath=no sys_lib_dlsearch_path_spec='/boot/home/config/lib /boot/common/lib /boot/system/lib' hardcode_into_libs=yes ;; hpux9* | hpux10* | hpux11*) # Give a soname corresponding to the major version so that dld.sl refuses to # link against other versions. version_type=sunos need_lib_prefix=no need_version=no case $host_cpu in ia64*) shrext_cmds='.so' hardcode_into_libs=yes dynamic_linker="$host_os dld.so" shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes # Unless +noenvvar is specified. library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' if test 32 = "$HPUX_IA64_MODE"; then sys_lib_search_path_spec="/usr/lib/hpux32 /usr/local/lib/hpux32 /usr/local/lib" sys_lib_dlsearch_path_spec=/usr/lib/hpux32 else sys_lib_search_path_spec="/usr/lib/hpux64 /usr/local/lib/hpux64" sys_lib_dlsearch_path_spec=/usr/lib/hpux64 fi ;; hppa*64*) shrext_cmds='.sl' hardcode_into_libs=yes dynamic_linker="$host_os dld.sl" shlibpath_var=LD_LIBRARY_PATH # How should we handle SHLIB_PATH shlibpath_overrides_runpath=yes # Unless +noenvvar is specified. library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' sys_lib_search_path_spec="/usr/lib/pa20_64 /usr/ccs/lib/pa20_64" sys_lib_dlsearch_path_spec=$sys_lib_search_path_spec ;; *) shrext_cmds='.sl' dynamic_linker="$host_os dld.sl" shlibpath_var=SHLIB_PATH shlibpath_overrides_runpath=no # +s is required to enable SHLIB_PATH library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' ;; esac # HP-UX runs *really* slowly unless shared libraries are mode 555, ... postinstall_cmds='chmod 555 $lib' # or fails outright, so override atomically: install_override_mode=555 ;; interix[[3-9]]*) version_type=linux # correct to gnu/linux during the next big refactor need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' dynamic_linker='Interix 3.x ld.so.1 (PE, like ELF)' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=no hardcode_into_libs=yes ;; irix5* | irix6* | nonstopux*) case $host_os in nonstopux*) version_type=nonstopux ;; *) if test yes = "$lt_cv_prog_gnu_ld"; then version_type=linux # correct to gnu/linux during the next big refactor else version_type=irix fi ;; esac need_lib_prefix=no need_version=no soname_spec='$libname$release$shared_ext$major' library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$release$shared_ext $libname$shared_ext' case $host_os in irix5* | nonstopux*) libsuff= shlibsuff= ;; *) case $LD in # libtool.m4 will add one of these switches to LD *-32|*"-32 "|*-melf32bsmip|*"-melf32bsmip ") libsuff= shlibsuff= libmagic=32-bit;; *-n32|*"-n32 "|*-melf32bmipn32|*"-melf32bmipn32 ") libsuff=32 shlibsuff=N32 libmagic=N32;; *-64|*"-64 "|*-melf64bmip|*"-melf64bmip ") libsuff=64 shlibsuff=64 libmagic=64-bit;; *) libsuff= shlibsuff= libmagic=never-match;; esac ;; esac shlibpath_var=LD_LIBRARY${shlibsuff}_PATH shlibpath_overrides_runpath=no sys_lib_search_path_spec="/usr/lib$libsuff /lib$libsuff /usr/local/lib$libsuff" sys_lib_dlsearch_path_spec="/usr/lib$libsuff /lib$libsuff" hardcode_into_libs=yes ;; # No shared lib support for Linux oldld, aout, or coff. linux*oldld* | linux*aout* | linux*coff*) dynamic_linker=no ;; linux*android*) version_type=none # Android doesn't support versioned libraries. need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext' soname_spec='$libname$release$shared_ext' finish_cmds= shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes # This implies no fast_install, which is unacceptable. # Some rework will be needed to allow for fast_install # before this can be enabled. hardcode_into_libs=yes dynamic_linker='Android linker' # Don't embed -rpath directories since the linker doesn't support them. _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='-L$libdir' ;; # This must be glibc/ELF. linux* | k*bsd*-gnu | kopensolaris*-gnu | gnu*) version_type=linux # correct to gnu/linux during the next big refactor need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' finish_cmds='PATH="\$PATH:/sbin" ldconfig -n $libdir' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=no # Some binutils ld are patched to set DT_RUNPATH AC_CACHE_VAL([lt_cv_shlibpath_overrides_runpath], [lt_cv_shlibpath_overrides_runpath=no save_LDFLAGS=$LDFLAGS save_libdir=$libdir eval "libdir=/foo; wl=\"$_LT_TAGVAR(lt_prog_compiler_wl, $1)\"; \ LDFLAGS=\"\$LDFLAGS $_LT_TAGVAR(hardcode_libdir_flag_spec, $1)\"" AC_LINK_IFELSE([AC_LANG_PROGRAM([],[])], [AS_IF([ ($OBJDUMP -p conftest$ac_exeext) 2>/dev/null | grep "RUNPATH.*$libdir" >/dev/null], [lt_cv_shlibpath_overrides_runpath=yes])]) LDFLAGS=$save_LDFLAGS libdir=$save_libdir ]) shlibpath_overrides_runpath=$lt_cv_shlibpath_overrides_runpath # This implies no fast_install, which is unacceptable. # Some rework will be needed to allow for fast_install # before this can be enabled. hardcode_into_libs=yes # Ideally, we could use ldconfig to report *all* directores which are # searched for libraries, however this is still not possible. 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*nto* | *qnx*) version_type=qnx need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=no hardcode_into_libs=yes dynamic_linker='ldqnx.so' ;; openbsd* | bitrig*) version_type=sunos sys_lib_dlsearch_path_spec=/usr/lib need_lib_prefix=no if test -z "`echo __ELF__ | $CC -E - | $GREP __ELF__`"; then need_version=no else need_version=yes fi library_names_spec='$libname$release$shared_ext$versuffix $libname$shared_ext$versuffix' finish_cmds='PATH="\$PATH:/sbin" ldconfig -m $libdir' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes ;; os2*) libname_spec='$name' version_type=windows shrext_cmds=.dll need_version=no need_lib_prefix=no # OS/2 can only load a DLL with a base name of 8 characters or less. soname_spec='`test -n "$os2dllname" && libname="$os2dllname"; v=$($ECHO $release$versuffix | tr -d .-); n=$($ECHO $libname | cut -b -$((8 - ${#v})) | tr . _); $ECHO $n$v`$shared_ext' library_names_spec='${libname}_dll.$libext' dynamic_linker='OS/2 ld.exe' shlibpath_var=BEGINLIBPATH sys_lib_search_path_spec="/lib /usr/lib /usr/local/lib" sys_lib_dlsearch_path_spec=$sys_lib_search_path_spec postinstall_cmds='base_file=`basename \$file`~ dlpath=`$SHELL 2>&1 -c '\''. $dir/'\''\$base_file'\''i; $ECHO \$dlname'\''`~ dldir=$destdir/`dirname \$dlpath`~ test -d \$dldir || mkdir -p \$dldir~ $install_prog $dir/$dlname \$dldir/$dlname~ chmod a+x \$dldir/$dlname~ if test -n '\''$stripme'\'' && test -n '\''$striplib'\''; then eval '\''$striplib \$dldir/$dlname'\'' || exit \$?; fi' postuninstall_cmds='dldll=`$SHELL 2>&1 -c '\''. $file; $ECHO \$dlname'\''`~ dlpath=$dir/\$dldll~ $RM \$dlpath' ;; osf3* | osf4* | osf5*) version_type=osf need_lib_prefix=no need_version=no soname_spec='$libname$release$shared_ext$major' library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' shlibpath_var=LD_LIBRARY_PATH sys_lib_search_path_spec="/usr/shlib /usr/ccs/lib /usr/lib/cmplrs/cc /usr/lib /usr/local/lib /var/shlib" sys_lib_dlsearch_path_spec=$sys_lib_search_path_spec ;; rdos*) dynamic_linker=no ;; solaris*) version_type=linux # correct to gnu/linux during the next big refactor need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes hardcode_into_libs=yes # ldd complains unless libraries are executable postinstall_cmds='chmod +x $lib' ;; sunos4*) version_type=sunos library_names_spec='$libname$release$shared_ext$versuffix $libname$shared_ext$versuffix' finish_cmds='PATH="\$PATH:/usr/etc" ldconfig $libdir' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes if test yes = "$with_gnu_ld"; then need_lib_prefix=no fi need_version=yes ;; sysv4 | sysv4.3*) version_type=linux # correct to gnu/linux during the next big refactor library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' shlibpath_var=LD_LIBRARY_PATH case $host_vendor in sni) shlibpath_overrides_runpath=no need_lib_prefix=no runpath_var=LD_RUN_PATH ;; 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sni) lt_cv_file_magic_cmd='/bin/file' lt_cv_deplibs_check_method="file_magic ELF [[0-9]][[0-9]]*-bit [[LM]]SB dynamic lib" lt_cv_file_magic_test_file=/lib/libc.so ;; siemens) lt_cv_deplibs_check_method=pass_all ;; pc) lt_cv_deplibs_check_method=pass_all ;; esac ;; tpf*) lt_cv_deplibs_check_method=pass_all ;; os2*) lt_cv_deplibs_check_method=pass_all ;; esac ]) file_magic_glob= want_nocaseglob=no if test "$build" = "$host"; then case $host_os in mingw* | pw32*) if ( shopt | grep nocaseglob ) >/dev/null 2>&1; then want_nocaseglob=yes else file_magic_glob=`echo aAbBcCdDeEfFgGhHiIjJkKlLmMnNoOpPqQrRsStTuUvVwWxXyYzZ | $SED -e "s/\(..\)/s\/[[\1]]\/[[\1]]\/g;/g"` fi ;; esac fi file_magic_cmd=$lt_cv_file_magic_cmd deplibs_check_method=$lt_cv_deplibs_check_method test -z "$deplibs_check_method" && deplibs_check_method=unknown _LT_DECL([], [deplibs_check_method], [1], [Method to check whether dependent libraries are shared objects]) _LT_DECL([], [file_magic_cmd], [1], [Command to use when deplibs_check_method = "file_magic"]) _LT_DECL([], [file_magic_glob], [1], [How to find potential files when deplibs_check_method = "file_magic"]) _LT_DECL([], [want_nocaseglob], [1], [Find potential files using nocaseglob when deplibs_check_method = "file_magic"]) ])# _LT_CHECK_MAGIC_METHOD # LT_PATH_NM # ---------- # find the pathname to a BSD- or MS-compatible name lister AC_DEFUN([LT_PATH_NM], [AC_REQUIRE([AC_PROG_CC])dnl AC_CACHE_CHECK([for BSD- or MS-compatible name lister (nm)], lt_cv_path_NM, [if test -n "$NM"; then # Let the user override the test. lt_cv_path_NM=$NM else lt_nm_to_check=${ac_tool_prefix}nm if test -n "$ac_tool_prefix" && test "$build" = "$host"; then lt_nm_to_check="$lt_nm_to_check nm" fi for lt_tmp_nm in $lt_nm_to_check; do lt_save_ifs=$IFS; IFS=$PATH_SEPARATOR for ac_dir in $PATH /usr/ccs/bin/elf /usr/ccs/bin /usr/ucb /bin; do IFS=$lt_save_ifs test -z "$ac_dir" && ac_dir=. tmp_nm=$ac_dir/$lt_tmp_nm if test -f "$tmp_nm" || test -f "$tmp_nm$ac_exeext"; then # Check to see if the nm accepts a BSD-compat flag. # Adding the 'sed 1q' prevents false positives on HP-UX, which says: # nm: unknown option "B" ignored # Tru64's nm complains that /dev/null is an invalid object file # MSYS converts /dev/null to NUL, MinGW nm treats NUL as empty case $build_os in mingw*) lt_bad_file=conftest.nm/nofile ;; *) lt_bad_file=/dev/null ;; esac case `"$tmp_nm" -B $lt_bad_file 2>&1 | sed '1q'` in *$lt_bad_file* | *'Invalid file or object type'*) lt_cv_path_NM="$tmp_nm -B" break 2 ;; *) case `"$tmp_nm" -p /dev/null 2>&1 | sed '1q'` in */dev/null*) lt_cv_path_NM="$tmp_nm -p" break 2 ;; *) lt_cv_path_NM=${lt_cv_path_NM="$tmp_nm"} # keep the first match, but continue # so that we can try to find one that supports BSD flags ;; esac ;; esac fi done IFS=$lt_save_ifs done : ${lt_cv_path_NM=no} fi]) if test no != "$lt_cv_path_NM"; then NM=$lt_cv_path_NM else # Didn't find any BSD compatible name lister, look for dumpbin. if test -n "$DUMPBIN"; then : # Let the user override the test. else AC_CHECK_TOOLS(DUMPBIN, [dumpbin "link -dump"], :) case `$DUMPBIN -symbols -headers /dev/null 2>&1 | sed '1q'` in *COFF*) DUMPBIN="$DUMPBIN -symbols -headers" ;; *) DUMPBIN=: ;; esac fi AC_SUBST([DUMPBIN]) if test : != "$DUMPBIN"; then NM=$DUMPBIN fi fi test -z "$NM" && NM=nm AC_SUBST([NM]) _LT_DECL([], [NM], [1], [A BSD- or MS-compatible name lister])dnl AC_CACHE_CHECK([the name lister ($NM) interface], [lt_cv_nm_interface], [lt_cv_nm_interface="BSD nm" echo "int some_variable = 0;" > conftest.$ac_ext (eval echo "\"\$as_me:$LINENO: $ac_compile\"" >&AS_MESSAGE_LOG_FD) (eval "$ac_compile" 2>conftest.err) cat conftest.err >&AS_MESSAGE_LOG_FD (eval echo "\"\$as_me:$LINENO: $NM \\\"conftest.$ac_objext\\\"\"" >&AS_MESSAGE_LOG_FD) (eval "$NM \"conftest.$ac_objext\"" 2>conftest.err > conftest.out) cat conftest.err >&AS_MESSAGE_LOG_FD (eval echo "\"\$as_me:$LINENO: output\"" >&AS_MESSAGE_LOG_FD) cat conftest.out >&AS_MESSAGE_LOG_FD if $GREP 'External.*some_variable' conftest.out > /dev/null; then lt_cv_nm_interface="MS dumpbin" fi rm -f conftest*]) ])# LT_PATH_NM # Old names: AU_ALIAS([AM_PROG_NM], [LT_PATH_NM]) AU_ALIAS([AC_PROG_NM], [LT_PATH_NM]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AM_PROG_NM], []) dnl AC_DEFUN([AC_PROG_NM], []) # _LT_CHECK_SHAREDLIB_FROM_LINKLIB # -------------------------------- # how to determine the name of the shared library # associated with a specific link library. # -- PORTME fill in with the dynamic library characteristics m4_defun([_LT_CHECK_SHAREDLIB_FROM_LINKLIB], [m4_require([_LT_DECL_EGREP]) m4_require([_LT_DECL_OBJDUMP]) m4_require([_LT_DECL_DLLTOOL]) AC_CACHE_CHECK([how to associate runtime and link libraries], lt_cv_sharedlib_from_linklib_cmd, [lt_cv_sharedlib_from_linklib_cmd='unknown' case $host_os in cygwin* | mingw* | pw32* | cegcc*) # two different shell functions defined in ltmain.sh; # decide which one to use based on capabilities of $DLLTOOL case `$DLLTOOL --help 2>&1` in *--identify-strict*) lt_cv_sharedlib_from_linklib_cmd=func_cygming_dll_for_implib ;; *) lt_cv_sharedlib_from_linklib_cmd=func_cygming_dll_for_implib_fallback ;; esac ;; *) # fallback: assume linklib IS sharedlib lt_cv_sharedlib_from_linklib_cmd=$ECHO ;; esac ]) sharedlib_from_linklib_cmd=$lt_cv_sharedlib_from_linklib_cmd test -z "$sharedlib_from_linklib_cmd" && sharedlib_from_linklib_cmd=$ECHO _LT_DECL([], [sharedlib_from_linklib_cmd], [1], [Command to associate shared and link libraries]) ])# _LT_CHECK_SHAREDLIB_FROM_LINKLIB # _LT_PATH_MANIFEST_TOOL # ---------------------- # locate the manifest tool m4_defun([_LT_PATH_MANIFEST_TOOL], [AC_CHECK_TOOL(MANIFEST_TOOL, mt, :) test -z "$MANIFEST_TOOL" && MANIFEST_TOOL=mt AC_CACHE_CHECK([if $MANIFEST_TOOL is a manifest tool], [lt_cv_path_mainfest_tool], [lt_cv_path_mainfest_tool=no echo "$as_me:$LINENO: $MANIFEST_TOOL '-?'" >&AS_MESSAGE_LOG_FD $MANIFEST_TOOL '-?' 2>conftest.err > conftest.out cat conftest.err >&AS_MESSAGE_LOG_FD if $GREP 'Manifest Tool' conftest.out > /dev/null; then lt_cv_path_mainfest_tool=yes fi rm -f conftest*]) if test yes != "$lt_cv_path_mainfest_tool"; then MANIFEST_TOOL=: fi _LT_DECL([], [MANIFEST_TOOL], [1], [Manifest tool])dnl ])# _LT_PATH_MANIFEST_TOOL # _LT_DLL_DEF_P([FILE]) # --------------------- # True iff FILE is a Windows DLL '.def' file. # Keep in sync with func_dll_def_p in the libtool script AC_DEFUN([_LT_DLL_DEF_P], [dnl test DEF = "`$SED -n dnl -e '\''s/^[[ ]]*//'\'' dnl Strip leading whitespace -e '\''/^\(;.*\)*$/d'\'' dnl Delete empty lines and comments -e '\''s/^\(EXPORTS\|LIBRARY\)\([[ ]].*\)*$/DEF/p'\'' dnl -e q dnl Only consider the first "real" line $1`" dnl ])# _LT_DLL_DEF_P # LT_LIB_M # -------- # check for math library AC_DEFUN([LT_LIB_M], [AC_REQUIRE([AC_CANONICAL_HOST])dnl LIBM= case $host in *-*-beos* | *-*-cegcc* | *-*-cygwin* | *-*-haiku* | *-*-pw32* | *-*-darwin*) # These system don't have libm, or don't need it ;; *-ncr-sysv4.3*) AC_CHECK_LIB(mw, _mwvalidcheckl, LIBM=-lmw) AC_CHECK_LIB(m, cos, LIBM="$LIBM -lm") ;; *) AC_CHECK_LIB(m, cos, LIBM=-lm) ;; esac AC_SUBST([LIBM]) ])# LT_LIB_M # Old name: AU_ALIAS([AC_CHECK_LIBM], [LT_LIB_M]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AC_CHECK_LIBM], []) # _LT_COMPILER_NO_RTTI([TAGNAME]) # ------------------------------- m4_defun([_LT_COMPILER_NO_RTTI], [m4_require([_LT_TAG_COMPILER])dnl _LT_TAGVAR(lt_prog_compiler_no_builtin_flag, $1)= if test yes = "$GCC"; then case $cc_basename in nvcc*) _LT_TAGVAR(lt_prog_compiler_no_builtin_flag, $1)=' -Xcompiler -fno-builtin' ;; *) _LT_TAGVAR(lt_prog_compiler_no_builtin_flag, $1)=' -fno-builtin' ;; esac _LT_COMPILER_OPTION([if $compiler supports -fno-rtti -fno-exceptions], lt_cv_prog_compiler_rtti_exceptions, [-fno-rtti -fno-exceptions], [], [_LT_TAGVAR(lt_prog_compiler_no_builtin_flag, $1)="$_LT_TAGVAR(lt_prog_compiler_no_builtin_flag, $1) -fno-rtti -fno-exceptions"]) fi _LT_TAGDECL([no_builtin_flag], [lt_prog_compiler_no_builtin_flag], [1], [Compiler flag to turn off builtin functions]) ])# _LT_COMPILER_NO_RTTI # _LT_CMD_GLOBAL_SYMBOLS # ---------------------- m4_defun([_LT_CMD_GLOBAL_SYMBOLS], [AC_REQUIRE([AC_CANONICAL_HOST])dnl AC_REQUIRE([AC_PROG_CC])dnl AC_REQUIRE([AC_PROG_AWK])dnl AC_REQUIRE([LT_PATH_NM])dnl AC_REQUIRE([LT_PATH_LD])dnl m4_require([_LT_DECL_SED])dnl m4_require([_LT_DECL_EGREP])dnl m4_require([_LT_TAG_COMPILER])dnl # Check for command to grab the raw symbol name followed by C symbol from nm. AC_MSG_CHECKING([command to parse $NM output from $compiler object]) AC_CACHE_VAL([lt_cv_sys_global_symbol_pipe], [ # These are sane defaults that work on at least a few old systems. # [They come from Ultrix. What could be older than Ultrix?!! ;)] # Character class describing NM global symbol codes. symcode='[[BCDEGRST]]' # Regexp to match symbols that can be accessed directly from C. sympat='\([[_A-Za-z]][[_A-Za-z0-9]]*\)' # Define system-specific variables. case $host_os in aix*) symcode='[[BCDT]]' ;; cygwin* | mingw* | pw32* | cegcc*) symcode='[[ABCDGISTW]]' ;; hpux*) if test ia64 = "$host_cpu"; then symcode='[[ABCDEGRST]]' fi ;; irix* | nonstopux*) symcode='[[BCDEGRST]]' ;; osf*) symcode='[[BCDEGQRST]]' ;; solaris*) symcode='[[BDRT]]' ;; sco3.2v5*) symcode='[[DT]]' ;; sysv4.2uw2*) symcode='[[DT]]' ;; sysv5* | sco5v6* | unixware* | OpenUNIX*) symcode='[[ABDT]]' ;; sysv4) symcode='[[DFNSTU]]' ;; esac # If we're using GNU nm, then use its standard symbol codes. case `$NM -V 2>&1` in *GNU* | *'with BFD'*) symcode='[[ABCDGIRSTW]]' ;; esac if test "$lt_cv_nm_interface" = "MS dumpbin"; then # Gets list of data symbols to import. lt_cv_sys_global_symbol_to_import="sed -n -e 's/^I .* \(.*\)$/\1/p'" # Adjust the below global symbol transforms to fixup imported variables. lt_cdecl_hook=" -e 's/^I .* \(.*\)$/extern __declspec(dllimport) char \1;/p'" lt_c_name_hook=" -e 's/^I .* \(.*\)$/ {\"\1\", (void *) 0},/p'" lt_c_name_lib_hook="\ -e 's/^I .* \(lib.*\)$/ {\"\1\", (void *) 0},/p'\ -e 's/^I .* \(.*\)$/ {\"lib\1\", (void *) 0},/p'" else # Disable hooks by default. lt_cv_sys_global_symbol_to_import= lt_cdecl_hook= lt_c_name_hook= lt_c_name_lib_hook= fi # Transform an extracted symbol line into a proper C declaration. # Some systems (esp. on ia64) link data and code symbols differently, # so use this general approach. lt_cv_sys_global_symbol_to_cdecl="sed -n"\ $lt_cdecl_hook\ " -e 's/^T .* \(.*\)$/extern int \1();/p'"\ " -e 's/^$symcode$symcode* .* \(.*\)$/extern char \1;/p'" # Transform an extracted symbol line into symbol name and symbol address lt_cv_sys_global_symbol_to_c_name_address="sed -n"\ $lt_c_name_hook\ " -e 's/^: \(.*\) .*$/ {\"\1\", (void *) 0},/p'"\ " -e 's/^$symcode$symcode* .* \(.*\)$/ {\"\1\", (void *) \&\1},/p'" # Transform an extracted symbol line into symbol name with lib prefix and # symbol address. lt_cv_sys_global_symbol_to_c_name_address_lib_prefix="sed -n"\ $lt_c_name_lib_hook\ " -e 's/^: \(.*\) .*$/ {\"\1\", (void *) 0},/p'"\ " -e 's/^$symcode$symcode* .* \(lib.*\)$/ {\"\1\", (void *) \&\1},/p'"\ " -e 's/^$symcode$symcode* .* \(.*\)$/ {\"lib\1\", (void *) \&\1},/p'" # Handle CRLF in mingw tool chain opt_cr= case $build_os in mingw*) opt_cr=`$ECHO 'x\{0,1\}' | tr x '\015'` # option cr in regexp ;; esac # Try without a prefix underscore, then with it. for ac_symprfx in "" "_"; do # Transform symcode, sympat, and symprfx into a raw symbol and a C symbol. symxfrm="\\1 $ac_symprfx\\2 \\2" # Write the raw and C identifiers. if test "$lt_cv_nm_interface" = "MS dumpbin"; then # Fake it for dumpbin and say T for any non-static function, # D for any global variable and I for any imported variable. # Also find C++ and __fastcall symbols from MSVC++, # which start with @ or ?. lt_cv_sys_global_symbol_pipe="$AWK ['"\ " {last_section=section; section=\$ 3};"\ " /^COFF SYMBOL TABLE/{for(i in hide) delete hide[i]};"\ " /Section length .*#relocs.*(pick any)/{hide[last_section]=1};"\ " /^ *Symbol name *: /{split(\$ 0,sn,\":\"); si=substr(sn[2],2)};"\ " /^ *Type *: code/{print \"T\",si,substr(si,length(prfx))};"\ " /^ *Type *: data/{print \"I\",si,substr(si,length(prfx))};"\ " \$ 0!~/External *\|/{next};"\ " / 0+ UNDEF /{next}; / UNDEF \([^|]\)*()/{next};"\ " {if(hide[section]) next};"\ " {f=\"D\"}; \$ 0~/\(\).*\|/{f=\"T\"};"\ " {split(\$ 0,a,/\||\r/); split(a[2],s)};"\ " s[1]~/^[@?]/{print f,s[1],s[1]; next};"\ " s[1]~prfx {split(s[1],t,\"@\"); print f,t[1],substr(t[1],length(prfx))}"\ " ' prfx=^$ac_symprfx]" else lt_cv_sys_global_symbol_pipe="sed -n -e 's/^.*[[ ]]\($symcode$symcode*\)[[ ]][[ ]]*$ac_symprfx$sympat$opt_cr$/$symxfrm/p'" fi lt_cv_sys_global_symbol_pipe="$lt_cv_sys_global_symbol_pipe | sed '/ __gnu_lto/d'" # Check to see that the pipe works correctly. pipe_works=no rm -f conftest* cat > conftest.$ac_ext <<_LT_EOF #ifdef __cplusplus extern "C" { #endif char nm_test_var; void nm_test_func(void); void nm_test_func(void){} #ifdef __cplusplus } #endif int main(){nm_test_var='a';nm_test_func();return(0);} _LT_EOF if AC_TRY_EVAL(ac_compile); then # Now try to grab the symbols. nlist=conftest.nm if AC_TRY_EVAL(NM conftest.$ac_objext \| "$lt_cv_sys_global_symbol_pipe" \> $nlist) && test -s "$nlist"; then # Try sorting and uniquifying the output. if sort "$nlist" | uniq > "$nlist"T; then mv -f "$nlist"T "$nlist" else rm -f "$nlist"T fi # Make sure that we snagged all the symbols we need. if $GREP ' nm_test_var$' "$nlist" >/dev/null; then if $GREP ' nm_test_func$' "$nlist" >/dev/null; then cat <<_LT_EOF > conftest.$ac_ext /* Keep this code in sync between libtool.m4, ltmain, lt_system.h, and tests. */ #if defined _WIN32 || defined __CYGWIN__ || defined _WIN32_WCE /* DATA imports from DLLs on WIN32 can't be const, because runtime relocations are performed -- see ld's documentation on pseudo-relocs. */ # define LT@&t@_DLSYM_CONST #elif defined __osf__ /* This system does not cope well with relocations in const data. */ # define LT@&t@_DLSYM_CONST #else # define LT@&t@_DLSYM_CONST const #endif #ifdef __cplusplus extern "C" { #endif _LT_EOF # Now generate the symbol file. eval "$lt_cv_sys_global_symbol_to_cdecl"' < "$nlist" | $GREP -v main >> conftest.$ac_ext' cat <<_LT_EOF >> conftest.$ac_ext /* The mapping between symbol names and symbols. */ LT@&t@_DLSYM_CONST struct { const char *name; void *address; } lt__PROGRAM__LTX_preloaded_symbols[[]] = { { "@PROGRAM@", (void *) 0 }, _LT_EOF $SED "s/^$symcode$symcode* .* \(.*\)$/ {\"\1\", (void *) \&\1},/" < "$nlist" | $GREP -v main >> conftest.$ac_ext cat <<\_LT_EOF >> conftest.$ac_ext {0, (void *) 0} }; /* This works around a problem in FreeBSD linker */ #ifdef FREEBSD_WORKAROUND static const void *lt_preloaded_setup() { return lt__PROGRAM__LTX_preloaded_symbols; } #endif #ifdef __cplusplus } #endif _LT_EOF # Now try linking the two files. mv conftest.$ac_objext conftstm.$ac_objext lt_globsym_save_LIBS=$LIBS lt_globsym_save_CFLAGS=$CFLAGS LIBS=conftstm.$ac_objext CFLAGS="$CFLAGS$_LT_TAGVAR(lt_prog_compiler_no_builtin_flag, $1)" if AC_TRY_EVAL(ac_link) && test -s conftest$ac_exeext; then pipe_works=yes fi LIBS=$lt_globsym_save_LIBS CFLAGS=$lt_globsym_save_CFLAGS else echo "cannot find nm_test_func in $nlist" >&AS_MESSAGE_LOG_FD fi else echo "cannot find nm_test_var in $nlist" >&AS_MESSAGE_LOG_FD fi else echo "cannot run $lt_cv_sys_global_symbol_pipe" >&AS_MESSAGE_LOG_FD fi else echo "$progname: failed program was:" >&AS_MESSAGE_LOG_FD cat conftest.$ac_ext >&5 fi rm -rf conftest* conftst* # Do not use the global_symbol_pipe unless it works. if test yes = "$pipe_works"; then break else lt_cv_sys_global_symbol_pipe= fi done ]) if test -z "$lt_cv_sys_global_symbol_pipe"; then lt_cv_sys_global_symbol_to_cdecl= fi if test -z "$lt_cv_sys_global_symbol_pipe$lt_cv_sys_global_symbol_to_cdecl"; then AC_MSG_RESULT(failed) else AC_MSG_RESULT(ok) fi # Response file support. if test "$lt_cv_nm_interface" = "MS dumpbin"; then nm_file_list_spec='@' elif $NM --help 2>/dev/null | grep '[[@]]FILE' >/dev/null; then nm_file_list_spec='@' fi _LT_DECL([global_symbol_pipe], [lt_cv_sys_global_symbol_pipe], [1], [Take the output of nm and produce a listing of raw symbols and C names]) _LT_DECL([global_symbol_to_cdecl], [lt_cv_sys_global_symbol_to_cdecl], [1], [Transform the output of nm in a proper C declaration]) _LT_DECL([global_symbol_to_import], [lt_cv_sys_global_symbol_to_import], [1], [Transform the output of nm into a list of symbols to manually relocate]) _LT_DECL([global_symbol_to_c_name_address], [lt_cv_sys_global_symbol_to_c_name_address], [1], [Transform the output of nm in a C name address pair]) _LT_DECL([global_symbol_to_c_name_address_lib_prefix], [lt_cv_sys_global_symbol_to_c_name_address_lib_prefix], [1], [Transform the output of nm in a C name address pair when lib prefix is needed]) _LT_DECL([nm_interface], [lt_cv_nm_interface], [1], [The name lister interface]) _LT_DECL([], [nm_file_list_spec], [1], [Specify filename containing input files for $NM]) ]) # _LT_CMD_GLOBAL_SYMBOLS # _LT_COMPILER_PIC([TAGNAME]) # --------------------------- m4_defun([_LT_COMPILER_PIC], [m4_require([_LT_TAG_COMPILER])dnl _LT_TAGVAR(lt_prog_compiler_wl, $1)= _LT_TAGVAR(lt_prog_compiler_pic, $1)= _LT_TAGVAR(lt_prog_compiler_static, $1)= m4_if([$1], [CXX], [ # C++ specific cases for pic, static, wl, etc. if test yes = "$GXX"; then _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_static, $1)='-static' case $host_os in aix*) # All AIX code is PIC. if test ia64 = "$host_cpu"; then # AIX 5 now supports IA64 processor _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' fi _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; amigaos*) case $host_cpu in powerpc) # see comment about AmigaOS4 .so support _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; m68k) # FIXME: we need at least 68020 code to build shared libraries, but # adding the '-m68020' flag to GCC prevents building anything better, # like '-m68040'. _LT_TAGVAR(lt_prog_compiler_pic, $1)='-m68020 -resident32 -malways-restore-a4' ;; esac ;; beos* | irix5* | irix6* | nonstopux* | osf3* | osf4* | osf5*) # PIC is the default for these OSes. ;; mingw* | cygwin* | os2* | pw32* | cegcc*) # This hack is so that the source file can tell whether it is being # built for inclusion in a dll (and should export symbols for example). # Although the cygwin gcc ignores -fPIC, still need this for old-style # (--disable-auto-import) libraries m4_if([$1], [GCJ], [], [_LT_TAGVAR(lt_prog_compiler_pic, $1)='-DDLL_EXPORT']) case $host_os in os2*) _LT_TAGVAR(lt_prog_compiler_static, $1)='$wl-static' ;; esac ;; darwin* | rhapsody*) # PIC is the default on this platform # Common symbols not allowed in MH_DYLIB files _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fno-common' ;; *djgpp*) # DJGPP does not support shared libraries at all _LT_TAGVAR(lt_prog_compiler_pic, $1)= ;; haiku*) # PIC is the default for Haiku. # The "-static" flag exists, but is broken. _LT_TAGVAR(lt_prog_compiler_static, $1)= ;; interix[[3-9]]*) # Interix 3.x gcc -fpic/-fPIC options generate broken code. # Instead, we relocate shared libraries at runtime. ;; sysv4*MP*) if test -d /usr/nec; then _LT_TAGVAR(lt_prog_compiler_pic, $1)=-Kconform_pic fi ;; hpux*) # PIC is the default for 64-bit PA HP-UX, but not for 32-bit # PA HP-UX. On IA64 HP-UX, PIC is the default but the pic flag # sets the default TLS model and affects inlining. case $host_cpu in hppa*64*) ;; *) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; esac ;; *qnx* | *nto*) # QNX uses GNU C++, but need to define -shared option too, otherwise # it will coredump. _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC -shared' ;; *) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; esac else case $host_os in aix[[4-9]]*) # All AIX code is PIC. if test ia64 = "$host_cpu"; then # AIX 5 now supports IA64 processor _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' else _LT_TAGVAR(lt_prog_compiler_static, $1)='-bnso -bI:/lib/syscalls.exp' fi ;; chorus*) case $cc_basename in cxch68*) # Green Hills C++ Compiler # _LT_TAGVAR(lt_prog_compiler_static, $1)="--no_auto_instantiation -u __main -u __premain -u _abort -r $COOL_DIR/lib/libOrb.a $MVME_DIR/lib/CC/libC.a $MVME_DIR/lib/classix/libcx.s.a" ;; esac ;; mingw* | cygwin* | os2* | pw32* | cegcc*) # This hack is so that the source file can tell whether it is being # built for inclusion in a dll (and should export symbols for example). m4_if([$1], [GCJ], [], [_LT_TAGVAR(lt_prog_compiler_pic, $1)='-DDLL_EXPORT']) ;; dgux*) case $cc_basename in ec++*) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' ;; ghcx*) # Green Hills C++ Compiler _LT_TAGVAR(lt_prog_compiler_pic, $1)='-pic' ;; *) ;; esac ;; freebsd* | dragonfly*) # FreeBSD uses GNU C++ ;; hpux9* | hpux10* | hpux11*) case $cc_basename in CC*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_static, $1)='$wl-a ${wl}archive' if test ia64 != "$host_cpu"; then _LT_TAGVAR(lt_prog_compiler_pic, $1)='+Z' fi ;; aCC*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_static, $1)='$wl-a ${wl}archive' case $host_cpu in hppa*64*|ia64*) # +Z the default ;; *) _LT_TAGVAR(lt_prog_compiler_pic, $1)='+Z' ;; esac ;; *) ;; esac ;; interix*) # This is c89, which is MS Visual C++ (no shared libs) # Anyone wants to do a port? ;; irix5* | irix6* | nonstopux*) case $cc_basename in CC*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_static, $1)='-non_shared' # CC pic flag -KPIC is the default. ;; *) ;; esac ;; linux* | k*bsd*-gnu | kopensolaris*-gnu | gnu*) case $cc_basename in KCC*) # KAI C++ Compiler _LT_TAGVAR(lt_prog_compiler_wl, $1)='--backend -Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; ecpc* ) # old Intel C++ for x86_64, which still supported -KPIC. _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-static' ;; icpc* ) # Intel C++, used to be incompatible with GCC. # ICC 10 doesn't accept -KPIC any more. _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-static' ;; pgCC* | pgcpp*) # Portland Group C++ compiler _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fpic' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; cxx*) # Compaq C++ # Make sure the PIC flag is empty. It appears that all Alpha # Linux and Compaq Tru64 Unix objects are PIC. _LT_TAGVAR(lt_prog_compiler_pic, $1)= _LT_TAGVAR(lt_prog_compiler_static, $1)='-non_shared' ;; xlc* | xlC* | bgxl[[cC]]* | mpixl[[cC]]*) # IBM XL 8.0, 9.0 on PPC and BlueGene _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-qpic' _LT_TAGVAR(lt_prog_compiler_static, $1)='-qstaticlink' ;; *) case `$CC -V 2>&1 | sed 5q` in *Sun\ C*) # Sun C++ 5.9 _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Qoption ld ' ;; esac ;; esac ;; lynxos*) ;; m88k*) ;; mvs*) case $cc_basename in cxx*) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-W c,exportall' ;; *) ;; esac ;; netbsd*) ;; *qnx* | *nto*) # QNX uses GNU C++, but need to define -shared option too, otherwise # it will coredump. _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC -shared' ;; osf3* | osf4* | osf5*) case $cc_basename in KCC*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='--backend -Wl,' ;; RCC*) # Rational C++ 2.4.1 _LT_TAGVAR(lt_prog_compiler_pic, $1)='-pic' ;; cxx*) # Digital/Compaq C++ _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' # Make sure the PIC flag is empty. It appears that all Alpha # Linux and Compaq Tru64 Unix objects are PIC. _LT_TAGVAR(lt_prog_compiler_pic, $1)= _LT_TAGVAR(lt_prog_compiler_static, $1)='-non_shared' ;; *) ;; esac ;; psos*) ;; solaris*) case $cc_basename in CC* | sunCC*) # Sun C++ 4.2, 5.x and Centerline C++ _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Qoption ld ' ;; gcx*) # Green Hills C++ Compiler _LT_TAGVAR(lt_prog_compiler_pic, $1)='-PIC' ;; *) ;; esac ;; sunos4*) case $cc_basename in CC*) # Sun C++ 4.x _LT_TAGVAR(lt_prog_compiler_pic, $1)='-pic' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; lcc*) # Lucid _LT_TAGVAR(lt_prog_compiler_pic, $1)='-pic' ;; *) ;; esac ;; sysv5* | unixware* | sco3.2v5* | sco5v6* | OpenUNIX*) case $cc_basename in CC*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; esac ;; tandem*) case $cc_basename in NCC*) # NonStop-UX NCC 3.20 _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' ;; *) ;; esac ;; vxworks*) ;; *) _LT_TAGVAR(lt_prog_compiler_can_build_shared, $1)=no ;; esac fi ], [ if test yes = "$GCC"; then _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_static, $1)='-static' case $host_os in aix*) # All AIX code is PIC. if test ia64 = "$host_cpu"; then # AIX 5 now supports IA64 processor _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' fi _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; amigaos*) case $host_cpu in powerpc) # see comment about AmigaOS4 .so support _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; m68k) # FIXME: we need at least 68020 code to build shared libraries, but # adding the '-m68020' flag to GCC prevents building anything better, # like '-m68040'. _LT_TAGVAR(lt_prog_compiler_pic, $1)='-m68020 -resident32 -malways-restore-a4' ;; esac ;; beos* | irix5* | irix6* | nonstopux* | osf3* | osf4* | osf5*) # PIC is the default for these OSes. ;; mingw* | cygwin* | pw32* | os2* | cegcc*) # This hack is so that the source file can tell whether it is being # built for inclusion in a dll (and should export symbols for example). # Although the cygwin gcc ignores -fPIC, still need this for old-style # (--disable-auto-import) libraries m4_if([$1], [GCJ], [], [_LT_TAGVAR(lt_prog_compiler_pic, $1)='-DDLL_EXPORT']) case $host_os in os2*) _LT_TAGVAR(lt_prog_compiler_static, $1)='$wl-static' ;; esac ;; darwin* | rhapsody*) # PIC is the default on this platform # Common symbols not allowed in MH_DYLIB files _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fno-common' ;; haiku*) # PIC is the default for Haiku. # The "-static" flag exists, but is broken. _LT_TAGVAR(lt_prog_compiler_static, $1)= ;; hpux*) # PIC is the default for 64-bit PA HP-UX, but not for 32-bit # PA HP-UX. On IA64 HP-UX, PIC is the default but the pic flag # sets the default TLS model and affects inlining. case $host_cpu in hppa*64*) # +Z the default ;; *) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; esac ;; interix[[3-9]]*) # Interix 3.x gcc -fpic/-fPIC options generate broken code. # Instead, we relocate shared libraries at runtime. ;; msdosdjgpp*) # Just because we use GCC doesn't mean we suddenly get shared libraries # on systems that don't support them. _LT_TAGVAR(lt_prog_compiler_can_build_shared, $1)=no enable_shared=no ;; *nto* | *qnx*) # QNX uses GNU C++, but need to define -shared option too, otherwise # it will coredump. _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC -shared' ;; sysv4*MP*) if test -d /usr/nec; then _LT_TAGVAR(lt_prog_compiler_pic, $1)=-Kconform_pic fi ;; *) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; esac case $cc_basename in nvcc*) # Cuda Compiler Driver 2.2 _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Xlinker ' if test -n "$_LT_TAGVAR(lt_prog_compiler_pic, $1)"; then _LT_TAGVAR(lt_prog_compiler_pic, $1)="-Xcompiler $_LT_TAGVAR(lt_prog_compiler_pic, $1)" fi ;; esac else # PORTME Check for flag to pass linker flags through the system compiler. case $host_os in aix*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' if test ia64 = "$host_cpu"; then # AIX 5 now supports IA64 processor _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' else _LT_TAGVAR(lt_prog_compiler_static, $1)='-bnso -bI:/lib/syscalls.exp' fi ;; darwin* | rhapsody*) # PIC is the default on this platform # Common symbols not allowed in MH_DYLIB files _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fno-common' case $cc_basename in nagfor*) # NAG Fortran compiler _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,-Wl,,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-PIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; esac ;; mingw* | cygwin* | pw32* | os2* | cegcc*) # This hack is so that the source file can tell whether it is being # built for inclusion in a dll (and should export symbols for example). m4_if([$1], [GCJ], [], [_LT_TAGVAR(lt_prog_compiler_pic, $1)='-DDLL_EXPORT']) case $host_os in os2*) _LT_TAGVAR(lt_prog_compiler_static, $1)='$wl-static' ;; esac ;; hpux9* | hpux10* | hpux11*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' # PIC is the default for IA64 HP-UX and 64-bit HP-UX, but # not for PA HP-UX. case $host_cpu in hppa*64*|ia64*) # +Z the default ;; *) _LT_TAGVAR(lt_prog_compiler_pic, $1)='+Z' ;; esac # Is there a better lt_prog_compiler_static that works with the bundled CC? _LT_TAGVAR(lt_prog_compiler_static, $1)='$wl-a ${wl}archive' ;; irix5* | irix6* | nonstopux*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' # PIC (with -KPIC) is the default. _LT_TAGVAR(lt_prog_compiler_static, $1)='-non_shared' ;; linux* | k*bsd*-gnu | kopensolaris*-gnu | gnu*) case $cc_basename in # old Intel for x86_64, which still supported -KPIC. ecc*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-static' ;; # icc used to be incompatible with GCC. # ICC 10 doesn't accept -KPIC any more. icc* | ifort*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-static' ;; # Lahey Fortran 8.1. lf95*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='--shared' _LT_TAGVAR(lt_prog_compiler_static, $1)='--static' ;; nagfor*) # NAG Fortran compiler _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,-Wl,,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-PIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; tcc*) # Fabrice Bellard et al's Tiny C Compiler _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-static' ;; pgcc* | pgf77* | pgf90* | pgf95* | pgfortran*) # Portland Group compilers (*not* the Pentium gcc compiler, # which looks to be a dead project) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fpic' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; ccc*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' # All Alpha code is PIC. _LT_TAGVAR(lt_prog_compiler_static, $1)='-non_shared' ;; xl* | bgxl* | bgf* | mpixl*) # IBM XL C 8.0/Fortran 10.1, 11.1 on PPC and BlueGene _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-qpic' _LT_TAGVAR(lt_prog_compiler_static, $1)='-qstaticlink' ;; *) case `$CC -V 2>&1 | sed 5q` in *Sun\ Ceres\ Fortran* | *Sun*Fortran*\ [[1-7]].* | *Sun*Fortran*\ 8.[[0-3]]*) # Sun Fortran 8.3 passes all unrecognized flags to the linker _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' _LT_TAGVAR(lt_prog_compiler_wl, $1)='' ;; *Sun\ F* | *Sun*Fortran*) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Qoption ld ' ;; *Sun\ C*) # Sun C 5.9 _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' ;; *Intel*\ [[CF]]*Compiler*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-static' ;; *Portland\ Group*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fpic' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; esac ;; esac ;; newsos6) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; *nto* | *qnx*) # QNX uses GNU C++, but need to define -shared option too, otherwise # it will coredump. _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC -shared' ;; osf3* | osf4* | osf5*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' # All OSF/1 code is PIC. _LT_TAGVAR(lt_prog_compiler_static, $1)='-non_shared' ;; rdos*) _LT_TAGVAR(lt_prog_compiler_static, $1)='-non_shared' ;; solaris*) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' case $cc_basename in f77* | f90* | f95* | sunf77* | sunf90* | sunf95*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Qoption ld ';; *) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,';; esac ;; sunos4*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Qoption ld ' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-PIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; sysv4 | sysv4.2uw2* | sysv4.3*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; sysv4*MP*) if test -d /usr/nec; then _LT_TAGVAR(lt_prog_compiler_pic, $1)='-Kconform_pic' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' fi ;; sysv5* | unixware* | sco3.2v5* | sco5v6* | OpenUNIX*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; unicos*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_can_build_shared, $1)=no ;; uts4*) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-pic' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; *) _LT_TAGVAR(lt_prog_compiler_can_build_shared, $1)=no ;; esac fi ]) case $host_os in # For platforms that do not support PIC, -DPIC is meaningless: *djgpp*) _LT_TAGVAR(lt_prog_compiler_pic, $1)= ;; *) _LT_TAGVAR(lt_prog_compiler_pic, $1)="$_LT_TAGVAR(lt_prog_compiler_pic, $1)@&t@m4_if([$1],[],[ -DPIC],[m4_if([$1],[CXX],[ -DPIC],[])])" ;; esac AC_CACHE_CHECK([for $compiler option to produce PIC], [_LT_TAGVAR(lt_cv_prog_compiler_pic, $1)], [_LT_TAGVAR(lt_cv_prog_compiler_pic, $1)=$_LT_TAGVAR(lt_prog_compiler_pic, $1)]) _LT_TAGVAR(lt_prog_compiler_pic, $1)=$_LT_TAGVAR(lt_cv_prog_compiler_pic, $1) # # Check to make sure the PIC flag actually works. # if test -n "$_LT_TAGVAR(lt_prog_compiler_pic, $1)"; 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AC_CACHE_CHECK([whether the $host_os linker accepts -exported_symbol], [lt_cv_irix_exported_symbol], [save_LDFLAGS=$LDFLAGS LDFLAGS="$LDFLAGS -shared $wl-exported_symbol ${wl}foo $wl-update_registry $wl/dev/null" AC_LINK_IFELSE( [AC_LANG_SOURCE( [AC_LANG_CASE([C], [[int foo (void) { return 0; }]], [C++], [[int foo (void) { return 0; }]], [Fortran 77], [[ subroutine foo end]], [Fortran], [[ subroutine foo end]])])], [lt_cv_irix_exported_symbol=yes], [lt_cv_irix_exported_symbol=no]) LDFLAGS=$save_LDFLAGS]) if test yes = "$lt_cv_irix_exported_symbol"; then _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname `test -n "$verstring" && func_echo_all "$wl-set_version $wl$verstring"` $wl-update_registry $wl$output_objdir/so_locations $wl-exports_file $wl$export_symbols -o $lib' fi else _LT_TAGVAR(archive_cmds, $1)='$CC -shared $libobjs $deplibs $compiler_flags -soname $soname `test -n "$verstring" && func_echo_all "-set_version $verstring"` -update_registry $output_objdir/so_locations -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -shared $libobjs $deplibs $compiler_flags -soname $soname `test -n "$verstring" && func_echo_all "-set_version $verstring"` -update_registry $output_objdir/so_locations -exports_file $export_symbols -o $lib' fi _LT_TAGVAR(archive_cmds_need_lc, $1)='no' _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl-rpath $wl$libdir' _LT_TAGVAR(hardcode_libdir_separator, $1)=: _LT_TAGVAR(inherit_rpath, $1)=yes _LT_TAGVAR(link_all_deplibs, $1)=yes ;; linux*) case $cc_basename in tcc*) # Fabrice Bellard et al's Tiny C Compiler _LT_TAGVAR(ld_shlibs, $1)=yes _LT_TAGVAR(archive_cmds, $1)='$CC -shared $pic_flag -o $lib $libobjs $deplibs $compiler_flags' ;; esac ;; netbsd*) if echo __ELF__ | $CC -E - | $GREP __ELF__ >/dev/null; then _LT_TAGVAR(archive_cmds, $1)='$LD -Bshareable -o $lib $libobjs $deplibs $linker_flags' # a.out else _LT_TAGVAR(archive_cmds, $1)='$LD -shared -o $lib $libobjs $deplibs $linker_flags' # ELF fi _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='-R$libdir' _LT_TAGVAR(hardcode_direct, $1)=yes _LT_TAGVAR(hardcode_shlibpath_var, $1)=no ;; newsos6) _LT_TAGVAR(archive_cmds, $1)='$LD -G -h $soname -o $lib $libobjs $deplibs $linker_flags' _LT_TAGVAR(hardcode_direct, $1)=yes _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl-rpath $wl$libdir' _LT_TAGVAR(hardcode_libdir_separator, $1)=: _LT_TAGVAR(hardcode_shlibpath_var, $1)=no ;; *nto* | *qnx*) ;; openbsd* | bitrig*) if test -f /usr/libexec/ld.so; then _LT_TAGVAR(hardcode_direct, $1)=yes _LT_TAGVAR(hardcode_shlibpath_var, $1)=no _LT_TAGVAR(hardcode_direct_absolute, $1)=yes if test -z "`echo __ELF__ | $CC -E - | $GREP __ELF__`"; then _LT_TAGVAR(archive_cmds, $1)='$CC -shared $pic_flag -o $lib $libobjs $deplibs $compiler_flags' _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -shared $pic_flag -o $lib $libobjs $deplibs $compiler_flags $wl-retain-symbols-file,$export_symbols' _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl-rpath,$libdir' _LT_TAGVAR(export_dynamic_flag_spec, $1)='$wl-E' else _LT_TAGVAR(archive_cmds, $1)='$CC -shared $pic_flag -o $lib $libobjs $deplibs $compiler_flags' _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl-rpath,$libdir' fi else _LT_TAGVAR(ld_shlibs, $1)=no fi ;; os2*) _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='-L$libdir' _LT_TAGVAR(hardcode_minus_L, $1)=yes _LT_TAGVAR(allow_undefined_flag, $1)=unsupported shrext_cmds=.dll _LT_TAGVAR(archive_cmds, $1)='$ECHO "LIBRARY ${soname%$shared_ext} INITINSTANCE TERMINSTANCE" > $output_objdir/$libname.def~ $ECHO "DESCRIPTION \"$libname\"" >> $output_objdir/$libname.def~ $ECHO "DATA MULTIPLE NONSHARED" >> $output_objdir/$libname.def~ $ECHO EXPORTS >> $output_objdir/$libname.def~ emxexp $libobjs | $SED /"_DLL_InitTerm"/d >> $output_objdir/$libname.def~ $CC -Zdll -Zcrtdll -o $output_objdir/$soname $libobjs $deplibs $compiler_flags $output_objdir/$libname.def~ emximp -o $lib $output_objdir/$libname.def' _LT_TAGVAR(archive_expsym_cmds, $1)='$ECHO "LIBRARY ${soname%$shared_ext} INITINSTANCE TERMINSTANCE" > $output_objdir/$libname.def~ $ECHO "DESCRIPTION \"$libname\"" >> $output_objdir/$libname.def~ $ECHO "DATA MULTIPLE NONSHARED" >> $output_objdir/$libname.def~ $ECHO EXPORTS >> $output_objdir/$libname.def~ prefix_cmds="$SED"~ if test EXPORTS = "`$SED 1q $export_symbols`"; then prefix_cmds="$prefix_cmds -e 1d"; fi~ prefix_cmds="$prefix_cmds -e \"s/^\(.*\)$/_\1/g\""~ cat $export_symbols | $prefix_cmds >> $output_objdir/$libname.def~ $CC -Zdll -Zcrtdll -o $output_objdir/$soname $libobjs $deplibs $compiler_flags $output_objdir/$libname.def~ emximp -o $lib $output_objdir/$libname.def' _LT_TAGVAR(old_archive_From_new_cmds, $1)='emximp -o $output_objdir/${libname}_dll.a $output_objdir/$libname.def' _LT_TAGVAR(enable_shared_with_static_runtimes, $1)=yes ;; osf3*) if test yes = "$GCC"; then _LT_TAGVAR(allow_undefined_flag, $1)=' $wl-expect_unresolved $wl\*' _LT_TAGVAR(archive_cmds, $1)='$CC -shared$allow_undefined_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname `test -n "$verstring" && func_echo_all "$wl-set_version $wl$verstring"` $wl-update_registry $wl$output_objdir/so_locations -o $lib' else _LT_TAGVAR(allow_undefined_flag, $1)=' -expect_unresolved \*' _LT_TAGVAR(archive_cmds, $1)='$CC -shared$allow_undefined_flag $libobjs $deplibs $compiler_flags -soname $soname `test -n "$verstring" && func_echo_all "-set_version $verstring"` -update_registry $output_objdir/so_locations -o $lib' fi _LT_TAGVAR(archive_cmds_need_lc, $1)='no' _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl-rpath $wl$libdir' _LT_TAGVAR(hardcode_libdir_separator, $1)=: ;; osf4* | osf5*) # as osf3* with the addition of -msym flag if test yes = "$GCC"; then _LT_TAGVAR(allow_undefined_flag, $1)=' $wl-expect_unresolved $wl\*' _LT_TAGVAR(archive_cmds, $1)='$CC -shared$allow_undefined_flag $pic_flag $libobjs $deplibs $compiler_flags $wl-msym $wl-soname $wl$soname `test -n "$verstring" && func_echo_all "$wl-set_version $wl$verstring"` $wl-update_registry $wl$output_objdir/so_locations -o $lib' _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl-rpath $wl$libdir' else _LT_TAGVAR(allow_undefined_flag, $1)=' -expect_unresolved \*' _LT_TAGVAR(archive_cmds, $1)='$CC -shared$allow_undefined_flag $libobjs $deplibs $compiler_flags -msym -soname $soname `test -n "$verstring" && func_echo_all "-set_version $verstring"` -update_registry $output_objdir/so_locations -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='for i in `cat $export_symbols`; do printf "%s %s\\n" -exported_symbol "\$i" >> $lib.exp; done; printf "%s\\n" "-hidden">> $lib.exp~ $CC -shared$allow_undefined_flag $wl-input $wl$lib.exp $compiler_flags $libobjs $deplibs -soname $soname `test -n "$verstring" && $ECHO "-set_version $verstring"` -update_registry $output_objdir/so_locations -o $lib~$RM $lib.exp' # Both c and cxx compiler support -rpath directly _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='-rpath $libdir' fi _LT_TAGVAR(archive_cmds_need_lc, $1)='no' _LT_TAGVAR(hardcode_libdir_separator, $1)=: ;; solaris*) _LT_TAGVAR(no_undefined_flag, $1)=' -z defs' if test yes = "$GCC"; then wlarc='$wl' _LT_TAGVAR(archive_cmds, $1)='$CC -shared $pic_flag $wl-z ${wl}text $wl-h $wl$soname -o $lib $libobjs $deplibs $compiler_flags' _LT_TAGVAR(archive_expsym_cmds, $1)='echo "{ global:" > $lib.exp~cat $export_symbols | $SED -e "s/\(.*\)/\1;/" >> $lib.exp~echo "local: *; };" >> $lib.exp~ $CC -shared $pic_flag $wl-z ${wl}text $wl-M $wl$lib.exp $wl-h $wl$soname -o $lib $libobjs $deplibs $compiler_flags~$RM $lib.exp' else case `$CC -V 2>&1` in *"Compilers 5.0"*) wlarc='' _LT_TAGVAR(archive_cmds, $1)='$LD -G$allow_undefined_flag -h $soname -o $lib $libobjs $deplibs $linker_flags' _LT_TAGVAR(archive_expsym_cmds, $1)='echo "{ global:" > $lib.exp~cat $export_symbols | $SED -e "s/\(.*\)/\1;/" >> $lib.exp~echo "local: *; };" >> $lib.exp~ $LD -G$allow_undefined_flag -M $lib.exp -h $soname -o $lib $libobjs $deplibs $linker_flags~$RM $lib.exp' ;; *) wlarc='$wl' _LT_TAGVAR(archive_cmds, $1)='$CC -G$allow_undefined_flag -h $soname -o $lib $libobjs $deplibs $compiler_flags' _LT_TAGVAR(archive_expsym_cmds, $1)='echo "{ global:" > $lib.exp~cat $export_symbols | $SED -e "s/\(.*\)/\1;/" >> $lib.exp~echo "local: *; };" >> $lib.exp~ $CC -G$allow_undefined_flag -M $lib.exp -h $soname -o $lib $libobjs $deplibs $compiler_flags~$RM $lib.exp' ;; esac fi _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='-R$libdir' _LT_TAGVAR(hardcode_shlibpath_var, $1)=no case $host_os in solaris2.[[0-5]] | solaris2.[[0-5]].*) ;; *) # The compiler driver will combine and reorder linker options, # but understands '-z linker_flag'. GCC discards it without '$wl', # but is careful enough not to reorder. # Supported since Solaris 2.6 (maybe 2.5.1?) if test yes = "$GCC"; then _LT_TAGVAR(whole_archive_flag_spec, $1)='$wl-z ${wl}allextract$convenience $wl-z ${wl}defaultextract' else _LT_TAGVAR(whole_archive_flag_spec, $1)='-z allextract$convenience -z defaultextract' fi ;; esac _LT_TAGVAR(link_all_deplibs, $1)=yes ;; sunos4*) if test sequent = "$host_vendor"; then # Use $CC to link under sequent, because it throws in some extra .o # files that make .init and .fini sections work. _LT_TAGVAR(archive_cmds, $1)='$CC -G $wl-h $soname -o $lib $libobjs $deplibs $compiler_flags' else _LT_TAGVAR(archive_cmds, $1)='$LD -assert pure-text -Bstatic -o $lib $libobjs $deplibs $linker_flags' fi _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='-L$libdir' _LT_TAGVAR(hardcode_direct, $1)=yes _LT_TAGVAR(hardcode_minus_L, $1)=yes _LT_TAGVAR(hardcode_shlibpath_var, $1)=no ;; sysv4) case $host_vendor in sni) _LT_TAGVAR(archive_cmds, $1)='$LD -G -h $soname -o $lib $libobjs $deplibs $linker_flags' _LT_TAGVAR(hardcode_direct, $1)=yes # is this really true??? ;; siemens) ## LD is ld it makes a PLAMLIB ## CC just makes a GrossModule. _LT_TAGVAR(archive_cmds, $1)='$LD -G -o $lib $libobjs $deplibs $linker_flags' _LT_TAGVAR(reload_cmds, $1)='$CC -r -o $output$reload_objs' _LT_TAGVAR(hardcode_direct, $1)=no ;; motorola) _LT_TAGVAR(archive_cmds, $1)='$LD -G -h $soname -o $lib $libobjs $deplibs $linker_flags' _LT_TAGVAR(hardcode_direct, $1)=no #Motorola manual says yes, but my tests say they lie ;; esac runpath_var='LD_RUN_PATH' _LT_TAGVAR(hardcode_shlibpath_var, $1)=no ;; sysv4.3*) _LT_TAGVAR(archive_cmds, $1)='$LD -G -h $soname -o $lib $libobjs $deplibs $linker_flags' _LT_TAGVAR(hardcode_shlibpath_var, $1)=no _LT_TAGVAR(export_dynamic_flag_spec, $1)='-Bexport' ;; sysv4*MP*) if test -d /usr/nec; then _LT_TAGVAR(archive_cmds, $1)='$LD -G -h $soname -o $lib $libobjs $deplibs $linker_flags' _LT_TAGVAR(hardcode_shlibpath_var, $1)=no runpath_var=LD_RUN_PATH hardcode_runpath_var=yes _LT_TAGVAR(ld_shlibs, $1)=yes fi ;; sysv4*uw2* | sysv5OpenUNIX* | sysv5UnixWare7.[[01]].[[10]]* | unixware7* | sco3.2v5.0.[[024]]*) _LT_TAGVAR(no_undefined_flag, $1)='$wl-z,text' _LT_TAGVAR(archive_cmds_need_lc, $1)=no _LT_TAGVAR(hardcode_shlibpath_var, $1)=no runpath_var='LD_RUN_PATH' if test yes = "$GCC"; then _LT_TAGVAR(archive_cmds, $1)='$CC -shared $wl-h,$soname -o $lib $libobjs $deplibs $compiler_flags' _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -shared $wl-Bexport:$export_symbols $wl-h,$soname -o $lib $libobjs $deplibs $compiler_flags' else _LT_TAGVAR(archive_cmds, $1)='$CC -G $wl-h,$soname -o $lib $libobjs $deplibs $compiler_flags' _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -G $wl-Bexport:$export_symbols $wl-h,$soname -o $lib $libobjs $deplibs $compiler_flags' fi ;; sysv5* | sco3.2v5* | sco5v6*) # Note: We CANNOT use -z defs as we might desire, because we do not # link with -lc, and that would cause any symbols used from libc to # always be unresolved, which means just about no library would # ever link correctly. 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These variables are subsequently used by _LT_CONFIG to write # the compiler configuration to 'libtool'. m4_defun([_LT_LANG_CXX_CONFIG], [m4_require([_LT_FILEUTILS_DEFAULTS])dnl m4_require([_LT_DECL_EGREP])dnl m4_require([_LT_PATH_MANIFEST_TOOL])dnl if test -n "$CXX" && ( test no != "$CXX" && ( (test g++ = "$CXX" && `g++ -v >/dev/null 2>&1` ) || (test g++ != "$CXX"))); then AC_PROG_CXXCPP else _lt_caught_CXX_error=yes fi AC_LANG_PUSH(C++) _LT_TAGVAR(archive_cmds_need_lc, $1)=no _LT_TAGVAR(allow_undefined_flag, $1)= _LT_TAGVAR(always_export_symbols, $1)=no _LT_TAGVAR(archive_expsym_cmds, $1)= _LT_TAGVAR(compiler_needs_object, $1)=no _LT_TAGVAR(export_dynamic_flag_spec, $1)= _LT_TAGVAR(hardcode_direct, $1)=no _LT_TAGVAR(hardcode_direct_absolute, $1)=no _LT_TAGVAR(hardcode_libdir_flag_spec, $1)= _LT_TAGVAR(hardcode_libdir_separator, $1)= _LT_TAGVAR(hardcode_minus_L, $1)=no _LT_TAGVAR(hardcode_shlibpath_var, $1)=unsupported _LT_TAGVAR(hardcode_automatic, $1)=no _LT_TAGVAR(inherit_rpath, $1)=no _LT_TAGVAR(module_cmds, $1)= _LT_TAGVAR(module_expsym_cmds, $1)= _LT_TAGVAR(link_all_deplibs, $1)=unknown _LT_TAGVAR(old_archive_cmds, $1)=$old_archive_cmds _LT_TAGVAR(reload_flag, $1)=$reload_flag _LT_TAGVAR(reload_cmds, $1)=$reload_cmds _LT_TAGVAR(no_undefined_flag, $1)= _LT_TAGVAR(whole_archive_flag_spec, $1)= _LT_TAGVAR(enable_shared_with_static_runtimes, $1)=no # Source file extension for C++ test sources. ac_ext=cpp # Object file extension for compiled C++ test sources. objext=o _LT_TAGVAR(objext, $1)=$objext # No sense in running all these tests if we already determined that # the CXX compiler isn't working. 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(MM) wlarc='$wl' # ancient GNU ld didn't support --whole-archive et. al. if eval "`$CC -print-prog-name=ld` --help 2>&1" | $GREP 'no-whole-archive' > /dev/null; then _LT_TAGVAR(whole_archive_flag_spec, $1)=$wlarc'--whole-archive$convenience '$wlarc'--no-whole-archive' else _LT_TAGVAR(whole_archive_flag_spec, $1)= fi else with_gnu_ld=no wlarc= # A generic and very simple default shared library creation # command for GNU C++ for the case where it uses the native # linker, instead of GNU ld. 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If -brtl is somewhere in LDFLAGS, we # have runtime linking enabled, and use it for executables. # For shared libraries, we enable/disable runtime linking # depending on the kind of the shared library created - # when "with_aix_soname,aix_use_runtimelinking" is: # "aix,no" lib.a(lib.so.V) shared, rtl:no, for executables # "aix,yes" lib.so shared, rtl:yes, for executables # lib.a static archive # "both,no" lib.so.V(shr.o) shared, rtl:yes # lib.a(lib.so.V) shared, rtl:no, for executables # "both,yes" lib.so.V(shr.o) shared, rtl:yes, for executables # lib.a(lib.so.V) shared, rtl:no # "svr4,*" lib.so.V(shr.o) shared, rtl:yes, for executables # lib.a static archive case $host_os in aix4.[[23]]|aix4.[[23]].*|aix[[5-9]]*) for ld_flag in $LDFLAGS; do case $ld_flag in *-brtl*) aix_use_runtimelinking=yes break ;; esac done if test svr4,no = "$with_aix_soname,$aix_use_runtimelinking"; then # With aix-soname=svr4, we create the lib.so.V shared archives only, # so we don't have lib.a shared libs to link our executables. # We have to force runtime linking in this case. aix_use_runtimelinking=yes LDFLAGS="$LDFLAGS -Wl,-brtl" fi ;; esac exp_sym_flag='-bexport' no_entry_flag='-bnoentry' fi # When large executables or shared objects are built, AIX ld can # have problems creating the table of contents. 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(KAI) C++ Compiler # KCC will only create a shared library if the output file # ends with ".so" (or ".sl" for HP-UX), so rename the library # to its proper name (with version) after linking. _LT_TAGVAR(archive_cmds, $1)='tempext=`echo $shared_ext | $SED -e '\''s/\([[^()0-9A-Za-z{}]]\)/\\\\\1/g'\''`; templib=`echo $lib | $SED -e "s/\$tempext\..*/.so/"`; $CC $predep_objects $libobjs $deplibs $postdep_objects $compiler_flags --soname $soname -o \$templib; mv \$templib $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='tempext=`echo $shared_ext | $SED -e '\''s/\([[^()0-9A-Za-z{}]]\)/\\\\\1/g'\''`; templib=`echo $lib | $SED -e "s/\$tempext\..*/.so/"`; $CC $predep_objects $libobjs $deplibs $postdep_objects $compiler_flags --soname $soname -o \$templib $wl-retain-symbols-file,$export_symbols; mv \$templib $lib' # Commands to make compiler produce verbose output that lists # what "hidden" libraries, object files and flags are used when # linking a shared library. # # There doesn't appear to be a way to prevent this compiler from # explicitly linking system object files so we need to strip them # from the output so that they don't get included in the library # dependencies. output_verbose_link_cmd='templist=`$CC $CFLAGS -v conftest.$objext -o libconftest$shared_ext 2>&1 | $GREP "ld"`; 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*) # Version 8.0 or newer tmp_idyn= case $host_cpu in ia64*) tmp_idyn=' -i_dynamic';; esac _LT_TAGVAR(archive_cmds, $1)='$CC -shared'"$tmp_idyn"' $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -shared'"$tmp_idyn"' $libobjs $deplibs $compiler_flags $wl-soname $wl$soname $wl-retain-symbols-file $wl$export_symbols -o $lib' ;; esac _LT_TAGVAR(archive_cmds_need_lc, $1)=no _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl-rpath,$libdir' _LT_TAGVAR(export_dynamic_flag_spec, $1)='$wl--export-dynamic' _LT_TAGVAR(whole_archive_flag_spec, $1)='$wl--whole-archive$convenience $wl--no-whole-archive' ;; pgCC* | pgcpp*) # Portland Group C++ compiler case `$CC -V` in *pgCC\ [[1-5]].* | *pgcpp\ [[1-5]].*) _LT_TAGVAR(prelink_cmds, $1)='tpldir=Template.dir~ rm -rf $tpldir~ $CC --prelink_objects --instantiation_dir $tpldir $objs $libobjs $compile_deplibs~ compile_command="$compile_command `find $tpldir -name \*.o | sort | $NL2SP`"' _LT_TAGVAR(old_archive_cmds, $1)='tpldir=Template.dir~ rm -rf $tpldir~ $CC --prelink_objects --instantiation_dir $tpldir $oldobjs$old_deplibs~ $AR $AR_FLAGS $oldlib$oldobjs$old_deplibs `find $tpldir -name \*.o | sort | $NL2SP`~ $RANLIB $oldlib' _LT_TAGVAR(archive_cmds, $1)='tpldir=Template.dir~ rm -rf $tpldir~ $CC --prelink_objects --instantiation_dir $tpldir $predep_objects $libobjs $deplibs $convenience $postdep_objects~ $CC -shared $pic_flag $predep_objects $libobjs $deplibs `find $tpldir -name \*.o | sort | $NL2SP` $postdep_objects $compiler_flags $wl-soname $wl$soname -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='tpldir=Template.dir~ rm -rf $tpldir~ $CC --prelink_objects --instantiation_dir $tpldir $predep_objects $libobjs $deplibs $convenience $postdep_objects~ $CC -shared $pic_flag $predep_objects $libobjs $deplibs `find $tpldir -name \*.o | sort | $NL2SP` $postdep_objects $compiler_flags $wl-soname $wl$soname $wl-retain-symbols-file $wl$export_symbols -o $lib' ;; *) # Version 6 and above use weak symbols _LT_TAGVAR(archive_cmds, $1)='$CC -shared $pic_flag $predep_objects $libobjs $deplibs $postdep_objects $compiler_flags $wl-soname $wl$soname -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -shared $pic_flag $predep_objects $libobjs $deplibs $postdep_objects $compiler_flags $wl-soname $wl$soname $wl-retain-symbols-file $wl$export_symbols -o $lib' ;; esac _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl--rpath $wl$libdir' _LT_TAGVAR(export_dynamic_flag_spec, $1)='$wl--export-dynamic' _LT_TAGVAR(whole_archive_flag_spec, $1)='$wl--whole-archive`for conv in $convenience\"\"; do test -n \"$conv\" && new_convenience=\"$new_convenience,$conv\"; done; func_echo_all \"$new_convenience\"` $wl--no-whole-archive' ;; cxx*) # Compaq C++ _LT_TAGVAR(archive_cmds, $1)='$CC -shared $predep_objects $libobjs $deplibs $postdep_objects $compiler_flags $wl-soname $wl$soname -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -shared $predep_objects $libobjs $deplibs $postdep_objects $compiler_flags $wl-soname $wl$soname -o $lib $wl-retain-symbols-file $wl$export_symbols' runpath_var=LD_RUN_PATH _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='-rpath $libdir' _LT_TAGVAR(hardcode_libdir_separator, $1)=: # Commands to make compiler produce verbose output that lists # what "hidden" libraries, object files and flags are used when # linking a shared library. # # There doesn't appear to be a way to prevent this compiler from # explicitly linking system object files so we need to strip them # from the output so that they don't get included in the library # dependencies. output_verbose_link_cmd='templist=`$CC -shared $CFLAGS -v conftest.$objext 2>&1 | $GREP "ld"`; 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These are needed # for certain cross-compile configurations and native mingw. m4_defun([_LT_PATH_CONVERSION_FUNCTIONS], [AC_REQUIRE([AC_CANONICAL_HOST])dnl AC_REQUIRE([AC_CANONICAL_BUILD])dnl AC_MSG_CHECKING([how to convert $build file names to $host format]) AC_CACHE_VAL(lt_cv_to_host_file_cmd, [case $host in *-*-mingw* ) case $build in *-*-mingw* ) # actually msys lt_cv_to_host_file_cmd=func_convert_file_msys_to_w32 ;; *-*-cygwin* ) lt_cv_to_host_file_cmd=func_convert_file_cygwin_to_w32 ;; * ) # otherwise, assume *nix lt_cv_to_host_file_cmd=func_convert_file_nix_to_w32 ;; esac ;; *-*-cygwin* ) case $build in *-*-mingw* ) # actually msys lt_cv_to_host_file_cmd=func_convert_file_msys_to_cygwin ;; *-*-cygwin* ) lt_cv_to_host_file_cmd=func_convert_file_noop ;; * ) # otherwise, assume *nix lt_cv_to_host_file_cmd=func_convert_file_nix_to_cygwin ;; esac ;; * ) # unhandled hosts (and "normal" native builds) lt_cv_to_host_file_cmd=func_convert_file_noop ;; esac ]) to_host_file_cmd=$lt_cv_to_host_file_cmd AC_MSG_RESULT([$lt_cv_to_host_file_cmd]) _LT_DECL([to_host_file_cmd], [lt_cv_to_host_file_cmd], [0], [convert $build file names to $host format])dnl AC_MSG_CHECKING([how to convert $build file names to toolchain format]) AC_CACHE_VAL(lt_cv_to_tool_file_cmd, [#assume ordinary cross tools, or native build. lt_cv_to_tool_file_cmd=func_convert_file_noop case $host in *-*-mingw* ) case $build in *-*-mingw* ) # actually msys lt_cv_to_tool_file_cmd=func_convert_file_msys_to_w32 ;; esac ;; esac ]) to_tool_file_cmd=$lt_cv_to_tool_file_cmd AC_MSG_RESULT([$lt_cv_to_tool_file_cmd]) _LT_DECL([to_tool_file_cmd], [lt_cv_to_tool_file_cmd], [0], [convert $build files to toolchain format])dnl ])# _LT_PATH_CONVERSION_FUNCTIONS gnuastro-0.2.33-8a3b/bootstrapped/m4/lib-prefix.m40000644000175000017500000002042213004436755016455 00000000000000# lib-prefix.m4 serial 7 (gettext-0.18) dnl Copyright (C) 2001-2005, 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl AC_LIB_ARG_WITH is synonymous to AC_ARG_WITH in autoconf-2.13, and dnl similar to AC_ARG_WITH in autoconf 2.52...2.57 except that is doesn't dnl require excessive bracketing. ifdef([AC_HELP_STRING], [AC_DEFUN([AC_LIB_ARG_WITH], [AC_ARG_WITH([$1],[[$2]],[$3],[$4])])], [AC_DEFUN([AC_][LIB_ARG_WITH], [AC_ARG_WITH([$1],[$2],[$3],[$4])])]) dnl AC_LIB_PREFIX adds to the CPPFLAGS and LDFLAGS the flags that are needed dnl to access previously installed libraries. The basic assumption is that dnl a user will want packages to use other packages he previously installed dnl with the same --prefix option. dnl This macro is not needed if only AC_LIB_LINKFLAGS is used to locate dnl libraries, but is otherwise very convenient. AC_DEFUN([AC_LIB_PREFIX], [ AC_BEFORE([$0], [AC_LIB_LINKFLAGS]) AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([AC_LIB_PREPARE_MULTILIB]) AC_REQUIRE([AC_LIB_PREPARE_PREFIX]) dnl By default, look in $includedir and $libdir. use_additional=yes AC_LIB_WITH_FINAL_PREFIX([ eval additional_includedir=\"$includedir\" eval additional_libdir=\"$libdir\" ]) AC_LIB_ARG_WITH([lib-prefix], [ --with-lib-prefix[=DIR] search for libraries in DIR/include and DIR/lib --without-lib-prefix don't search for libraries in includedir and libdir], [ if test "X$withval" = "Xno"; then use_additional=no else if test "X$withval" = "X"; then AC_LIB_WITH_FINAL_PREFIX([ eval additional_includedir=\"$includedir\" eval additional_libdir=\"$libdir\" ]) else additional_includedir="$withval/include" additional_libdir="$withval/$acl_libdirstem" fi fi ]) if test $use_additional = yes; then dnl Potentially add $additional_includedir to $CPPFLAGS. dnl But don't add it dnl 1. if it's the standard /usr/include, dnl 2. if it's already present in $CPPFLAGS, dnl 3. if it's /usr/local/include and we are using GCC on Linux, dnl 4. if it doesn't exist as a directory. if test "X$additional_includedir" != "X/usr/include"; then haveit= for x in $CPPFLAGS; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) if test "X$x" = "X-I$additional_includedir"; then haveit=yes break fi done if test -z "$haveit"; then if test "X$additional_includedir" = "X/usr/local/include"; then if test -n "$GCC"; then case $host_os in linux* | gnu* | k*bsd*-gnu) haveit=yes;; esac fi fi if test -z "$haveit"; then if test -d "$additional_includedir"; then dnl Really add $additional_includedir to $CPPFLAGS. CPPFLAGS="${CPPFLAGS}${CPPFLAGS:+ }-I$additional_includedir" fi fi fi fi dnl Potentially add $additional_libdir to $LDFLAGS. dnl But don't add it dnl 1. if it's the standard /usr/lib, dnl 2. if it's already present in $LDFLAGS, dnl 3. if it's /usr/local/lib and we are using GCC on Linux, dnl 4. if it doesn't exist as a directory. if test "X$additional_libdir" != "X/usr/$acl_libdirstem"; then haveit= for x in $LDFLAGS; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) if test "X$x" = "X-L$additional_libdir"; then haveit=yes break fi done if test -z "$haveit"; then if test "X$additional_libdir" = "X/usr/local/$acl_libdirstem"; then if test -n "$GCC"; then case $host_os in linux*) haveit=yes;; esac fi fi if test -z "$haveit"; then if test -d "$additional_libdir"; then dnl Really add $additional_libdir to $LDFLAGS. LDFLAGS="${LDFLAGS}${LDFLAGS:+ }-L$additional_libdir" fi fi fi fi fi ]) dnl AC_LIB_PREPARE_PREFIX creates variables acl_final_prefix, dnl acl_final_exec_prefix, containing the values to which $prefix and dnl $exec_prefix will expand at the end of the configure script. AC_DEFUN([AC_LIB_PREPARE_PREFIX], [ dnl Unfortunately, prefix and exec_prefix get only finally determined dnl at the end of configure. if test "X$prefix" = "XNONE"; then acl_final_prefix="$ac_default_prefix" else acl_final_prefix="$prefix" fi if test "X$exec_prefix" = "XNONE"; then acl_final_exec_prefix='${prefix}' else acl_final_exec_prefix="$exec_prefix" fi acl_save_prefix="$prefix" prefix="$acl_final_prefix" eval acl_final_exec_prefix=\"$acl_final_exec_prefix\" prefix="$acl_save_prefix" ]) dnl AC_LIB_WITH_FINAL_PREFIX([statement]) evaluates statement, with the dnl variables prefix and exec_prefix bound to the values they will have dnl at the end of the configure script. AC_DEFUN([AC_LIB_WITH_FINAL_PREFIX], [ acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" $1 exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" ]) dnl AC_LIB_PREPARE_MULTILIB creates dnl - a variable acl_libdirstem, containing the basename of the libdir, either dnl "lib" or "lib64" or "lib/64", dnl - a variable acl_libdirstem2, as a secondary possible value for dnl acl_libdirstem, either the same as acl_libdirstem or "lib/sparcv9" or dnl "lib/amd64". AC_DEFUN([AC_LIB_PREPARE_MULTILIB], [ dnl There is no formal standard regarding lib and lib64. dnl On glibc systems, the current practice is that on a system supporting dnl 32-bit and 64-bit instruction sets or ABIs, 64-bit libraries go under dnl $prefix/lib64 and 32-bit libraries go under $prefix/lib. We determine dnl the compiler's default mode by looking at the compiler's library search dnl path. If at least one of its elements ends in /lib64 or points to a dnl directory whose absolute pathname ends in /lib64, we assume a 64-bit ABI. dnl Otherwise we use the default, namely "lib". dnl On Solaris systems, the current practice is that on a system supporting dnl 32-bit and 64-bit instruction sets or ABIs, 64-bit libraries go under dnl $prefix/lib/64 (which is a symlink to either $prefix/lib/sparcv9 or dnl $prefix/lib/amd64) and 32-bit libraries go under $prefix/lib. AC_REQUIRE([AC_CANONICAL_HOST]) acl_libdirstem=lib acl_libdirstem2= case "$host_os" in solaris*) dnl See Solaris 10 Software Developer Collection > Solaris 64-bit Developer's Guide > The Development Environment dnl . dnl "Portable Makefiles should refer to any library directories using the 64 symbolic link." dnl But we want to recognize the sparcv9 or amd64 subdirectory also if the dnl symlink is missing, so we set acl_libdirstem2 too. AC_CACHE_CHECK([for 64-bit host], [gl_cv_solaris_64bit], [AC_EGREP_CPP([sixtyfour bits], [ #ifdef _LP64 sixtyfour bits #endif ], [gl_cv_solaris_64bit=yes], [gl_cv_solaris_64bit=no]) ]) if test $gl_cv_solaris_64bit = yes; then acl_libdirstem=lib/64 case "$host_cpu" in sparc*) acl_libdirstem2=lib/sparcv9 ;; i*86 | x86_64) acl_libdirstem2=lib/amd64 ;; esac fi ;; *) searchpath=`(LC_ALL=C $CC -print-search-dirs) 2>/dev/null | sed -n -e 's,^libraries: ,,p' | sed -e 's,^=,,'` if test -n "$searchpath"; then acl_save_IFS="${IFS= }"; IFS=":" for searchdir in $searchpath; do if test -d "$searchdir"; then case "$searchdir" in */lib64/ | */lib64 ) acl_libdirstem=lib64 ;; */../ | */.. ) # Better ignore directories of this form. They are misleading. ;; *) searchdir=`cd "$searchdir" && pwd` case "$searchdir" in */lib64 ) acl_libdirstem=lib64 ;; esac ;; esac fi done IFS="$acl_save_IFS" fi ;; esac test -n "$acl_libdirstem2" || acl_libdirstem2="$acl_libdirstem" ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/lib-link.m40000644000175000017500000010044313004436755016117 00000000000000# lib-link.m4 serial 26 (gettext-0.18.2) dnl Copyright (C) 2001-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. AC_PREREQ([2.54]) dnl AC_LIB_LINKFLAGS(name [, dependencies]) searches for libname and dnl the libraries corresponding to explicit and implicit dependencies. dnl Sets and AC_SUBSTs the LIB${NAME} and LTLIB${NAME} variables and dnl augments the CPPFLAGS variable. dnl Sets and AC_SUBSTs the LIB${NAME}_PREFIX variable to nonempty if libname dnl was found in ${LIB${NAME}_PREFIX}/$acl_libdirstem. AC_DEFUN([AC_LIB_LINKFLAGS], [ AC_REQUIRE([AC_LIB_PREPARE_PREFIX]) AC_REQUIRE([AC_LIB_RPATH]) pushdef([Name],[m4_translit([$1],[./+-], [____])]) pushdef([NAME],[m4_translit([$1],[abcdefghijklmnopqrstuvwxyz./+-], [ABCDEFGHIJKLMNOPQRSTUVWXYZ____])]) AC_CACHE_CHECK([how to link with lib[]$1], [ac_cv_lib[]Name[]_libs], [ AC_LIB_LINKFLAGS_BODY([$1], [$2]) ac_cv_lib[]Name[]_libs="$LIB[]NAME" ac_cv_lib[]Name[]_ltlibs="$LTLIB[]NAME" ac_cv_lib[]Name[]_cppflags="$INC[]NAME" ac_cv_lib[]Name[]_prefix="$LIB[]NAME[]_PREFIX" ]) LIB[]NAME="$ac_cv_lib[]Name[]_libs" LTLIB[]NAME="$ac_cv_lib[]Name[]_ltlibs" INC[]NAME="$ac_cv_lib[]Name[]_cppflags" LIB[]NAME[]_PREFIX="$ac_cv_lib[]Name[]_prefix" AC_LIB_APPENDTOVAR([CPPFLAGS], [$INC]NAME) AC_SUBST([LIB]NAME) AC_SUBST([LTLIB]NAME) AC_SUBST([LIB]NAME[_PREFIX]) dnl Also set HAVE_LIB[]NAME so that AC_LIB_HAVE_LINKFLAGS can reuse the dnl results of this search when this library appears as a dependency. HAVE_LIB[]NAME=yes popdef([NAME]) popdef([Name]) ]) dnl AC_LIB_HAVE_LINKFLAGS(name, dependencies, includes, testcode, [missing-message]) dnl searches for libname and the libraries corresponding to explicit and dnl implicit dependencies, together with the specified include files and dnl the ability to compile and link the specified testcode. The missing-message dnl defaults to 'no' and may contain additional hints for the user. dnl If found, it sets and AC_SUBSTs HAVE_LIB${NAME}=yes and the LIB${NAME} dnl and LTLIB${NAME} variables and augments the CPPFLAGS variable, and dnl #defines HAVE_LIB${NAME} to 1. Otherwise, it sets and AC_SUBSTs dnl HAVE_LIB${NAME}=no and LIB${NAME} and LTLIB${NAME} to empty. dnl Sets and AC_SUBSTs the LIB${NAME}_PREFIX variable to nonempty if libname dnl was found in ${LIB${NAME}_PREFIX}/$acl_libdirstem. AC_DEFUN([AC_LIB_HAVE_LINKFLAGS], [ AC_REQUIRE([AC_LIB_PREPARE_PREFIX]) AC_REQUIRE([AC_LIB_RPATH]) pushdef([Name],[m4_translit([$1],[./+-], [____])]) pushdef([NAME],[m4_translit([$1],[abcdefghijklmnopqrstuvwxyz./+-], [ABCDEFGHIJKLMNOPQRSTUVWXYZ____])]) dnl Search for lib[]Name and define LIB[]NAME, LTLIB[]NAME and INC[]NAME dnl accordingly. AC_LIB_LINKFLAGS_BODY([$1], [$2]) dnl Add $INC[]NAME to CPPFLAGS before performing the following checks, dnl because if the user has installed lib[]Name and not disabled its use dnl via --without-lib[]Name-prefix, he wants to use it. ac_save_CPPFLAGS="$CPPFLAGS" AC_LIB_APPENDTOVAR([CPPFLAGS], [$INC]NAME) AC_CACHE_CHECK([for lib[]$1], [ac_cv_lib[]Name], [ ac_save_LIBS="$LIBS" dnl If $LIB[]NAME contains some -l options, add it to the end of LIBS, dnl because these -l options might require -L options that are present in dnl LIBS. -l options benefit only from the -L options listed before it. dnl Otherwise, add it to the front of LIBS, because it may be a static dnl library that depends on another static library that is present in LIBS. dnl Static libraries benefit only from the static libraries listed after dnl it. case " $LIB[]NAME" in *" -l"*) LIBS="$LIBS $LIB[]NAME" ;; *) LIBS="$LIB[]NAME $LIBS" ;; esac AC_LINK_IFELSE( [AC_LANG_PROGRAM([[$3]], [[$4]])], [ac_cv_lib[]Name=yes], [ac_cv_lib[]Name='m4_if([$5], [], [no], [[$5]])']) LIBS="$ac_save_LIBS" ]) if test "$ac_cv_lib[]Name" = yes; then HAVE_LIB[]NAME=yes AC_DEFINE([HAVE_LIB]NAME, 1, [Define if you have the lib][$1 library.]) AC_MSG_CHECKING([how to link with lib[]$1]) AC_MSG_RESULT([$LIB[]NAME]) else HAVE_LIB[]NAME=no dnl If $LIB[]NAME didn't lead to a usable library, we don't need dnl $INC[]NAME either. CPPFLAGS="$ac_save_CPPFLAGS" LIB[]NAME= LTLIB[]NAME= LIB[]NAME[]_PREFIX= fi AC_SUBST([HAVE_LIB]NAME) AC_SUBST([LIB]NAME) AC_SUBST([LTLIB]NAME) AC_SUBST([LIB]NAME[_PREFIX]) popdef([NAME]) popdef([Name]) ]) dnl Determine the platform dependent parameters needed to use rpath: dnl acl_libext, dnl acl_shlibext, dnl acl_libname_spec, dnl acl_library_names_spec, dnl acl_hardcode_libdir_flag_spec, dnl acl_hardcode_libdir_separator, dnl acl_hardcode_direct, dnl acl_hardcode_minus_L. AC_DEFUN([AC_LIB_RPATH], [ dnl Tell automake >= 1.10 to complain if config.rpath is missing. m4_ifdef([AC_REQUIRE_AUX_FILE], [AC_REQUIRE_AUX_FILE([config.rpath])]) AC_REQUIRE([AC_PROG_CC]) dnl we use $CC, $GCC, $LDFLAGS AC_REQUIRE([AC_LIB_PROG_LD]) dnl we use $LD, $with_gnu_ld AC_REQUIRE([AC_CANONICAL_HOST]) dnl we use $host AC_REQUIRE([AC_CONFIG_AUX_DIR_DEFAULT]) dnl we use $ac_aux_dir AC_CACHE_CHECK([for shared library run path origin], [acl_cv_rpath], [ CC="$CC" GCC="$GCC" LDFLAGS="$LDFLAGS" LD="$LD" with_gnu_ld="$with_gnu_ld" \ ${CONFIG_SHELL-/bin/sh} "$ac_aux_dir/config.rpath" "$host" > conftest.sh . ./conftest.sh rm -f ./conftest.sh acl_cv_rpath=done ]) wl="$acl_cv_wl" acl_libext="$acl_cv_libext" acl_shlibext="$acl_cv_shlibext" acl_libname_spec="$acl_cv_libname_spec" acl_library_names_spec="$acl_cv_library_names_spec" acl_hardcode_libdir_flag_spec="$acl_cv_hardcode_libdir_flag_spec" acl_hardcode_libdir_separator="$acl_cv_hardcode_libdir_separator" acl_hardcode_direct="$acl_cv_hardcode_direct" acl_hardcode_minus_L="$acl_cv_hardcode_minus_L" dnl Determine whether the user wants rpath handling at all. AC_ARG_ENABLE([rpath], [ --disable-rpath do not hardcode runtime library paths], :, enable_rpath=yes) ]) dnl AC_LIB_FROMPACKAGE(name, package) dnl declares that libname comes from the given package. The configure file dnl will then not have a --with-libname-prefix option but a dnl --with-package-prefix option. Several libraries can come from the same dnl package. This declaration must occur before an AC_LIB_LINKFLAGS or similar dnl macro call that searches for libname. AC_DEFUN([AC_LIB_FROMPACKAGE], [ pushdef([NAME],[m4_translit([$1],[abcdefghijklmnopqrstuvwxyz./+-], [ABCDEFGHIJKLMNOPQRSTUVWXYZ____])]) define([acl_frompackage_]NAME, [$2]) popdef([NAME]) pushdef([PACK],[$2]) pushdef([PACKUP],[m4_translit(PACK,[abcdefghijklmnopqrstuvwxyz./+-], [ABCDEFGHIJKLMNOPQRSTUVWXYZ____])]) define([acl_libsinpackage_]PACKUP, m4_ifdef([acl_libsinpackage_]PACKUP, [m4_defn([acl_libsinpackage_]PACKUP)[, ]],)[lib$1]) popdef([PACKUP]) popdef([PACK]) ]) dnl AC_LIB_LINKFLAGS_BODY(name [, dependencies]) searches for libname and dnl the libraries corresponding to explicit and implicit dependencies. dnl Sets the LIB${NAME}, LTLIB${NAME} and INC${NAME} variables. dnl Also, sets the LIB${NAME}_PREFIX variable to nonempty if libname was found dnl in ${LIB${NAME}_PREFIX}/$acl_libdirstem. AC_DEFUN([AC_LIB_LINKFLAGS_BODY], [ AC_REQUIRE([AC_LIB_PREPARE_MULTILIB]) pushdef([NAME],[m4_translit([$1],[abcdefghijklmnopqrstuvwxyz./+-], [ABCDEFGHIJKLMNOPQRSTUVWXYZ____])]) pushdef([PACK],[m4_ifdef([acl_frompackage_]NAME, [acl_frompackage_]NAME, lib[$1])]) pushdef([PACKUP],[m4_translit(PACK,[abcdefghijklmnopqrstuvwxyz./+-], [ABCDEFGHIJKLMNOPQRSTUVWXYZ____])]) pushdef([PACKLIBS],[m4_ifdef([acl_frompackage_]NAME, [acl_libsinpackage_]PACKUP, lib[$1])]) dnl Autoconf >= 2.61 supports dots in --with options. pushdef([P_A_C_K],[m4_if(m4_version_compare(m4_defn([m4_PACKAGE_VERSION]),[2.61]),[-1],[m4_translit(PACK,[.],[_])],PACK)]) dnl By default, look in $includedir and $libdir. use_additional=yes AC_LIB_WITH_FINAL_PREFIX([ eval additional_includedir=\"$includedir\" eval additional_libdir=\"$libdir\" ]) AC_ARG_WITH(P_A_C_K[-prefix], [[ --with-]]P_A_C_K[[-prefix[=DIR] search for ]PACKLIBS[ in DIR/include and DIR/lib --without-]]P_A_C_K[[-prefix don't search for ]PACKLIBS[ in includedir and libdir]], [ if test "X$withval" = "Xno"; then use_additional=no else if test "X$withval" = "X"; then AC_LIB_WITH_FINAL_PREFIX([ eval additional_includedir=\"$includedir\" eval additional_libdir=\"$libdir\" ]) else additional_includedir="$withval/include" additional_libdir="$withval/$acl_libdirstem" if test "$acl_libdirstem2" != "$acl_libdirstem" \ && ! test -d "$withval/$acl_libdirstem"; then additional_libdir="$withval/$acl_libdirstem2" fi fi fi ]) dnl Search the library and its dependencies in $additional_libdir and dnl $LDFLAGS. Using breadth-first-seach. LIB[]NAME= LTLIB[]NAME= INC[]NAME= LIB[]NAME[]_PREFIX= dnl HAVE_LIB${NAME} is an indicator that LIB${NAME}, LTLIB${NAME} have been dnl computed. So it has to be reset here. HAVE_LIB[]NAME= rpathdirs= ltrpathdirs= names_already_handled= names_next_round='$1 $2' while test -n "$names_next_round"; do names_this_round="$names_next_round" names_next_round= for name in $names_this_round; do already_handled= for n in $names_already_handled; do if test "$n" = "$name"; then already_handled=yes break fi done if test -z "$already_handled"; then names_already_handled="$names_already_handled $name" dnl See if it was already located by an earlier AC_LIB_LINKFLAGS dnl or AC_LIB_HAVE_LINKFLAGS call. uppername=`echo "$name" | sed -e 'y|abcdefghijklmnopqrstuvwxyz./+-|ABCDEFGHIJKLMNOPQRSTUVWXYZ____|'` eval value=\"\$HAVE_LIB$uppername\" if test -n "$value"; then if test "$value" = yes; then eval value=\"\$LIB$uppername\" test -z "$value" || LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$value" eval value=\"\$LTLIB$uppername\" test -z "$value" || LTLIB[]NAME="${LTLIB[]NAME}${LTLIB[]NAME:+ }$value" else dnl An earlier call to AC_LIB_HAVE_LINKFLAGS has determined dnl that this library doesn't exist. So just drop it. : fi else dnl Search the library lib$name in $additional_libdir and $LDFLAGS dnl and the already constructed $LIBNAME/$LTLIBNAME. found_dir= found_la= found_so= found_a= eval libname=\"$acl_libname_spec\" # typically: libname=lib$name if test -n "$acl_shlibext"; then shrext=".$acl_shlibext" # typically: shrext=.so else shrext= fi if test $use_additional = yes; then dir="$additional_libdir" dnl The same code as in the loop below: dnl First look for a shared library. if test -n "$acl_shlibext"; then if test -f "$dir/$libname$shrext"; then found_dir="$dir" found_so="$dir/$libname$shrext" else if test "$acl_library_names_spec" = '$libname$shrext$versuffix'; then ver=`(cd "$dir" && \ for f in "$libname$shrext".*; do echo "$f"; done \ | sed -e "s,^$libname$shrext\\\\.,," \ | sort -t '.' -n -r -k1,1 -k2,2 -k3,3 -k4,4 -k5,5 \ | sed 1q ) 2>/dev/null` if test -n "$ver" && test -f "$dir/$libname$shrext.$ver"; then found_dir="$dir" found_so="$dir/$libname$shrext.$ver" fi else eval library_names=\"$acl_library_names_spec\" for f in $library_names; do if test -f "$dir/$f"; then found_dir="$dir" found_so="$dir/$f" break fi done fi fi fi dnl Then look for a static library. if test "X$found_dir" = "X"; then if test -f "$dir/$libname.$acl_libext"; then found_dir="$dir" found_a="$dir/$libname.$acl_libext" fi fi if test "X$found_dir" != "X"; then if test -f "$dir/$libname.la"; then found_la="$dir/$libname.la" fi fi fi if test "X$found_dir" = "X"; then for x in $LDFLAGS $LTLIB[]NAME; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) case "$x" in -L*) dir=`echo "X$x" | sed -e 's/^X-L//'` dnl First look for a shared library. if test -n "$acl_shlibext"; then if test -f "$dir/$libname$shrext"; then found_dir="$dir" found_so="$dir/$libname$shrext" else if test "$acl_library_names_spec" = '$libname$shrext$versuffix'; then ver=`(cd "$dir" && \ for f in "$libname$shrext".*; do echo "$f"; done \ | sed -e "s,^$libname$shrext\\\\.,," \ | sort -t '.' -n -r -k1,1 -k2,2 -k3,3 -k4,4 -k5,5 \ | sed 1q ) 2>/dev/null` if test -n "$ver" && test -f "$dir/$libname$shrext.$ver"; then found_dir="$dir" found_so="$dir/$libname$shrext.$ver" fi else eval library_names=\"$acl_library_names_spec\" for f in $library_names; do if test -f "$dir/$f"; then found_dir="$dir" found_so="$dir/$f" break fi done fi fi fi dnl Then look for a static library. if test "X$found_dir" = "X"; then if test -f "$dir/$libname.$acl_libext"; then found_dir="$dir" found_a="$dir/$libname.$acl_libext" fi fi if test "X$found_dir" != "X"; then if test -f "$dir/$libname.la"; then found_la="$dir/$libname.la" fi fi ;; esac if test "X$found_dir" != "X"; then break fi done fi if test "X$found_dir" != "X"; then dnl Found the library. LTLIB[]NAME="${LTLIB[]NAME}${LTLIB[]NAME:+ }-L$found_dir -l$name" if test "X$found_so" != "X"; then dnl Linking with a shared library. We attempt to hardcode its dnl directory into the executable's runpath, unless it's the dnl standard /usr/lib. if test "$enable_rpath" = no \ || test "X$found_dir" = "X/usr/$acl_libdirstem" \ || test "X$found_dir" = "X/usr/$acl_libdirstem2"; then dnl No hardcoding is needed. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$found_so" else dnl Use an explicit option to hardcode DIR into the resulting dnl binary. dnl Potentially add DIR to ltrpathdirs. dnl The ltrpathdirs will be appended to $LTLIBNAME at the end. haveit= for x in $ltrpathdirs; do if test "X$x" = "X$found_dir"; then haveit=yes break fi done if test -z "$haveit"; then ltrpathdirs="$ltrpathdirs $found_dir" fi dnl The hardcoding into $LIBNAME is system dependent. if test "$acl_hardcode_direct" = yes; then dnl Using DIR/libNAME.so during linking hardcodes DIR into the dnl resulting binary. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$found_so" else if test -n "$acl_hardcode_libdir_flag_spec" && test "$acl_hardcode_minus_L" = no; then dnl Use an explicit option to hardcode DIR into the resulting dnl binary. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$found_so" dnl Potentially add DIR to rpathdirs. dnl The rpathdirs will be appended to $LIBNAME at the end. haveit= for x in $rpathdirs; do if test "X$x" = "X$found_dir"; then haveit=yes break fi done if test -z "$haveit"; then rpathdirs="$rpathdirs $found_dir" fi else dnl Rely on "-L$found_dir". dnl But don't add it if it's already contained in the LDFLAGS dnl or the already constructed $LIBNAME haveit= for x in $LDFLAGS $LIB[]NAME; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) if test "X$x" = "X-L$found_dir"; then haveit=yes break fi done if test -z "$haveit"; then LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }-L$found_dir" fi if test "$acl_hardcode_minus_L" != no; then dnl FIXME: Not sure whether we should use dnl "-L$found_dir -l$name" or "-L$found_dir $found_so" dnl here. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$found_so" else dnl We cannot use $acl_hardcode_runpath_var and LD_RUN_PATH dnl here, because this doesn't fit in flags passed to the dnl compiler. So give up. No hardcoding. This affects only dnl very old systems. dnl FIXME: Not sure whether we should use dnl "-L$found_dir -l$name" or "-L$found_dir $found_so" dnl here. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }-l$name" fi fi fi fi else if test "X$found_a" != "X"; then dnl Linking with a static library. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$found_a" else dnl We shouldn't come here, but anyway it's good to have a dnl fallback. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }-L$found_dir -l$name" fi fi dnl Assume the include files are nearby. additional_includedir= case "$found_dir" in */$acl_libdirstem | */$acl_libdirstem/) basedir=`echo "X$found_dir" | sed -e 's,^X,,' -e "s,/$acl_libdirstem/"'*$,,'` if test "$name" = '$1'; then LIB[]NAME[]_PREFIX="$basedir" fi additional_includedir="$basedir/include" ;; */$acl_libdirstem2 | */$acl_libdirstem2/) basedir=`echo "X$found_dir" | sed -e 's,^X,,' -e "s,/$acl_libdirstem2/"'*$,,'` if test "$name" = '$1'; then LIB[]NAME[]_PREFIX="$basedir" fi additional_includedir="$basedir/include" ;; esac if test "X$additional_includedir" != "X"; then dnl Potentially add $additional_includedir to $INCNAME. dnl But don't add it dnl 1. if it's the standard /usr/include, dnl 2. if it's /usr/local/include and we are using GCC on Linux, dnl 3. if it's already present in $CPPFLAGS or the already dnl constructed $INCNAME, dnl 4. if it doesn't exist as a directory. if test "X$additional_includedir" != "X/usr/include"; then haveit= if test "X$additional_includedir" = "X/usr/local/include"; then if test -n "$GCC"; then case $host_os in linux* | gnu* | k*bsd*-gnu) haveit=yes;; esac fi fi if test -z "$haveit"; then for x in $CPPFLAGS $INC[]NAME; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) if test "X$x" = "X-I$additional_includedir"; then haveit=yes break fi done if test -z "$haveit"; then if test -d "$additional_includedir"; then dnl Really add $additional_includedir to $INCNAME. INC[]NAME="${INC[]NAME}${INC[]NAME:+ }-I$additional_includedir" fi fi fi fi fi dnl Look for dependencies. if test -n "$found_la"; then dnl Read the .la file. It defines the variables dnl dlname, library_names, old_library, dependency_libs, current, dnl age, revision, installed, dlopen, dlpreopen, libdir. save_libdir="$libdir" case "$found_la" in */* | *\\*) . "$found_la" ;; *) . "./$found_la" ;; esac libdir="$save_libdir" dnl We use only dependency_libs. for dep in $dependency_libs; do case "$dep" in -L*) additional_libdir=`echo "X$dep" | sed -e 's/^X-L//'` dnl Potentially add $additional_libdir to $LIBNAME and $LTLIBNAME. dnl But don't add it dnl 1. if it's the standard /usr/lib, dnl 2. if it's /usr/local/lib and we are using GCC on Linux, dnl 3. if it's already present in $LDFLAGS or the already dnl constructed $LIBNAME, dnl 4. if it doesn't exist as a directory. if test "X$additional_libdir" != "X/usr/$acl_libdirstem" \ && test "X$additional_libdir" != "X/usr/$acl_libdirstem2"; then haveit= if test "X$additional_libdir" = "X/usr/local/$acl_libdirstem" \ || test "X$additional_libdir" = "X/usr/local/$acl_libdirstem2"; then if test -n "$GCC"; then case $host_os in linux* | gnu* | k*bsd*-gnu) haveit=yes;; esac fi fi if test -z "$haveit"; then haveit= for x in $LDFLAGS $LIB[]NAME; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) if test "X$x" = "X-L$additional_libdir"; then haveit=yes break fi done if test -z "$haveit"; then if test -d "$additional_libdir"; then dnl Really add $additional_libdir to $LIBNAME. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }-L$additional_libdir" fi fi haveit= for x in $LDFLAGS $LTLIB[]NAME; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) if test "X$x" = "X-L$additional_libdir"; then haveit=yes break fi done if test -z "$haveit"; then if test -d "$additional_libdir"; then dnl Really add $additional_libdir to $LTLIBNAME. LTLIB[]NAME="${LTLIB[]NAME}${LTLIB[]NAME:+ }-L$additional_libdir" fi fi fi fi ;; -R*) dir=`echo "X$dep" | sed -e 's/^X-R//'` if test "$enable_rpath" != no; then dnl Potentially add DIR to rpathdirs. dnl The rpathdirs will be appended to $LIBNAME at the end. haveit= for x in $rpathdirs; do if test "X$x" = "X$dir"; then haveit=yes break fi done if test -z "$haveit"; then rpathdirs="$rpathdirs $dir" fi dnl Potentially add DIR to ltrpathdirs. dnl The ltrpathdirs will be appended to $LTLIBNAME at the end. haveit= for x in $ltrpathdirs; do if test "X$x" = "X$dir"; then haveit=yes break fi done if test -z "$haveit"; then ltrpathdirs="$ltrpathdirs $dir" fi fi ;; -l*) dnl Handle this in the next round. names_next_round="$names_next_round "`echo "X$dep" | sed -e 's/^X-l//'` ;; *.la) dnl Handle this in the next round. Throw away the .la's dnl directory; it is already contained in a preceding -L dnl option. names_next_round="$names_next_round "`echo "X$dep" | sed -e 's,^X.*/,,' -e 's,^lib,,' -e 's,\.la$,,'` ;; *) dnl Most likely an immediate library name. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$dep" LTLIB[]NAME="${LTLIB[]NAME}${LTLIB[]NAME:+ }$dep" ;; esac done fi else dnl Didn't find the library; assume it is in the system directories dnl known to the linker and runtime loader. (All the system dnl directories known to the linker should also be known to the dnl runtime loader, otherwise the system is severely misconfigured.) LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }-l$name" LTLIB[]NAME="${LTLIB[]NAME}${LTLIB[]NAME:+ }-l$name" fi fi fi done done if test "X$rpathdirs" != "X"; then if test -n "$acl_hardcode_libdir_separator"; then dnl Weird platform: only the last -rpath option counts, the user must dnl pass all path elements in one option. We can arrange that for a dnl single library, but not when more than one $LIBNAMEs are used. alldirs= for found_dir in $rpathdirs; do alldirs="${alldirs}${alldirs:+$acl_hardcode_libdir_separator}$found_dir" done dnl Note: acl_hardcode_libdir_flag_spec uses $libdir and $wl. acl_save_libdir="$libdir" libdir="$alldirs" eval flag=\"$acl_hardcode_libdir_flag_spec\" libdir="$acl_save_libdir" LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$flag" else dnl The -rpath options are cumulative. for found_dir in $rpathdirs; do acl_save_libdir="$libdir" libdir="$found_dir" eval flag=\"$acl_hardcode_libdir_flag_spec\" libdir="$acl_save_libdir" LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$flag" done fi fi if test "X$ltrpathdirs" != "X"; then dnl When using libtool, the option that works for both libraries and dnl executables is -R. The -R options are cumulative. for found_dir in $ltrpathdirs; do LTLIB[]NAME="${LTLIB[]NAME}${LTLIB[]NAME:+ }-R$found_dir" done fi popdef([P_A_C_K]) popdef([PACKLIBS]) popdef([PACKUP]) popdef([PACK]) popdef([NAME]) ]) dnl AC_LIB_APPENDTOVAR(VAR, CONTENTS) appends the elements of CONTENTS to VAR, dnl unless already present in VAR. dnl Works only for CPPFLAGS, not for LIB* variables because that sometimes dnl contains two or three consecutive elements that belong together. AC_DEFUN([AC_LIB_APPENDTOVAR], [ for element in [$2]; do haveit= for x in $[$1]; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) if test "X$x" = "X$element"; then haveit=yes break fi done if test -z "$haveit"; then [$1]="${[$1]}${[$1]:+ }$element" fi done ]) dnl For those cases where a variable contains several -L and -l options dnl referring to unknown libraries and directories, this macro determines the dnl necessary additional linker options for the runtime path. dnl AC_LIB_LINKFLAGS_FROM_LIBS([LDADDVAR], [LIBSVALUE], [USE-LIBTOOL]) dnl sets LDADDVAR to linker options needed together with LIBSVALUE. dnl If USE-LIBTOOL evaluates to non-empty, linking with libtool is assumed, dnl otherwise linking without libtool is assumed. AC_DEFUN([AC_LIB_LINKFLAGS_FROM_LIBS], [ AC_REQUIRE([AC_LIB_RPATH]) AC_REQUIRE([AC_LIB_PREPARE_MULTILIB]) $1= if test "$enable_rpath" != no; then if test -n "$acl_hardcode_libdir_flag_spec" && test "$acl_hardcode_minus_L" = no; then dnl Use an explicit option to hardcode directories into the resulting dnl binary. rpathdirs= next= for opt in $2; do if test -n "$next"; then dir="$next" dnl No need to hardcode the standard /usr/lib. if test "X$dir" != "X/usr/$acl_libdirstem" \ && test "X$dir" != "X/usr/$acl_libdirstem2"; then rpathdirs="$rpathdirs $dir" fi next= else case $opt in -L) next=yes ;; -L*) dir=`echo "X$opt" | sed -e 's,^X-L,,'` dnl No need to hardcode the standard /usr/lib. if test "X$dir" != "X/usr/$acl_libdirstem" \ && test "X$dir" != "X/usr/$acl_libdirstem2"; then rpathdirs="$rpathdirs $dir" fi next= ;; *) next= ;; esac fi done if test "X$rpathdirs" != "X"; then if test -n ""$3""; then dnl libtool is used for linking. Use -R options. for dir in $rpathdirs; do $1="${$1}${$1:+ }-R$dir" done else dnl The linker is used for linking directly. if test -n "$acl_hardcode_libdir_separator"; then dnl Weird platform: only the last -rpath option counts, the user dnl must pass all path elements in one option. alldirs= for dir in $rpathdirs; do alldirs="${alldirs}${alldirs:+$acl_hardcode_libdir_separator}$dir" done acl_save_libdir="$libdir" libdir="$alldirs" eval flag=\"$acl_hardcode_libdir_flag_spec\" libdir="$acl_save_libdir" $1="$flag" else dnl The -rpath options are cumulative. for dir in $rpathdirs; do acl_save_libdir="$libdir" libdir="$dir" eval flag=\"$acl_hardcode_libdir_flag_spec\" libdir="$acl_save_libdir" $1="${$1}${$1:+ }$flag" done fi fi fi fi fi AC_SUBST([$1]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/lib-ld.m40000644000175000017500000000714313004436755015564 00000000000000# lib-ld.m4 serial 6 dnl Copyright (C) 1996-2003, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Subroutines of libtool.m4, dnl with replacements s/_*LT_PATH/AC_LIB_PROG/ and s/lt_/acl_/ to avoid dnl collision with libtool.m4. dnl From libtool-2.4. Sets the variable with_gnu_ld to yes or no. AC_DEFUN([AC_LIB_PROG_LD_GNU], [AC_CACHE_CHECK([if the linker ($LD) is GNU ld], [acl_cv_prog_gnu_ld], [# I'd rather use --version here, but apparently some GNU lds only accept -v. case `$LD -v 2>&1 /dev/null 2>&1 \ && { (PATH='/bin:/bin'; FPATH=$PATH; sh -c :) >/dev/null 2>&1 \ || PATH_SEPARATOR=';' } fi ac_prog=ld if test "$GCC" = yes; then # Check if gcc -print-prog-name=ld gives a path. AC_MSG_CHECKING([for ld used by $CC]) case $host in *-*-mingw*) # gcc leaves a trailing carriage return which upsets mingw ac_prog=`($CC -print-prog-name=ld) 2>&5 | tr -d '\015'` ;; *) ac_prog=`($CC -print-prog-name=ld) 2>&5` ;; esac case $ac_prog in # Accept absolute paths. [[\\/]]* | ?:[[\\/]]*) re_direlt='/[[^/]][[^/]]*/\.\./' # Canonicalize the pathname of ld ac_prog=`echo "$ac_prog"| sed 's%\\\\%/%g'` while echo "$ac_prog" | grep "$re_direlt" > /dev/null 2>&1; do ac_prog=`echo $ac_prog| sed "s%$re_direlt%/%"` done test -z "$LD" && LD="$ac_prog" ;; "") # If it fails, then pretend we aren't using GCC. ac_prog=ld ;; *) # If it is relative, then search for the first ld in PATH. with_gnu_ld=unknown ;; esac elif test "$with_gnu_ld" = yes; then AC_MSG_CHECKING([for GNU ld]) else AC_MSG_CHECKING([for non-GNU ld]) fi AC_CACHE_VAL([acl_cv_path_LD], [if test -z "$LD"; then acl_save_ifs="$IFS"; IFS=$PATH_SEPARATOR for ac_dir in $PATH; do IFS="$acl_save_ifs" test -z "$ac_dir" && ac_dir=. if test -f "$ac_dir/$ac_prog" || test -f "$ac_dir/$ac_prog$ac_exeext"; then acl_cv_path_LD="$ac_dir/$ac_prog" # Check to see if the program is GNU ld. I'd rather use --version, # but apparently some variants of GNU ld only accept -v. # Break only if it was the GNU/non-GNU ld that we prefer. case `"$acl_cv_path_LD" -v 2>&1 , 1995. # Check whether LC_MESSAGES is available in . AC_DEFUN([gt_LC_MESSAGES], [ AC_CACHE_CHECK([for LC_MESSAGES], [gt_cv_val_LC_MESSAGES], [AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[return LC_MESSAGES]])], [gt_cv_val_LC_MESSAGES=yes], [gt_cv_val_LC_MESSAGES=no])]) if test $gt_cv_val_LC_MESSAGES = yes; then AC_DEFINE([HAVE_LC_MESSAGES], [1], [Define if your file defines LC_MESSAGES.]) fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/largefile.m40000644000175000017500000001233213004436755016347 00000000000000# Enable large files on systems where this is not the default. # Copyright 1992-1996, 1998-2016 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # The following implementation works around a problem in autoconf <= 2.69; # AC_SYS_LARGEFILE does not configure for large inodes on Mac OS X 10.5, # or configures them incorrectly in some cases. m4_version_prereq([2.70], [] ,[ # _AC_SYS_LARGEFILE_TEST_INCLUDES # ------------------------------- m4_define([_AC_SYS_LARGEFILE_TEST_INCLUDES], [@%:@include /* Check that off_t can represent 2**63 - 1 correctly. We can't simply define LARGE_OFF_T to be 9223372036854775807, since some C++ compilers masquerading as C compilers incorrectly reject 9223372036854775807. */ @%:@define LARGE_OFF_T (((off_t) 1 << 62) - 1 + ((off_t) 1 << 62)) int off_t_is_large[[(LARGE_OFF_T % 2147483629 == 721 && LARGE_OFF_T % 2147483647 == 1) ? 1 : -1]];[]dnl ]) # _AC_SYS_LARGEFILE_MACRO_VALUE(C-MACRO, VALUE, # CACHE-VAR, # DESCRIPTION, # PROLOGUE, [FUNCTION-BODY]) # -------------------------------------------------------- m4_define([_AC_SYS_LARGEFILE_MACRO_VALUE], [AC_CACHE_CHECK([for $1 value needed for large files], [$3], [while :; do m4_ifval([$6], [AC_LINK_IFELSE], [AC_COMPILE_IFELSE])( [AC_LANG_PROGRAM([$5], [$6])], [$3=no; break]) m4_ifval([$6], [AC_LINK_IFELSE], [AC_COMPILE_IFELSE])( [AC_LANG_PROGRAM([@%:@define $1 $2 $5], [$6])], [$3=$2; break]) $3=unknown break done]) case $$3 in #( no | unknown) ;; *) AC_DEFINE_UNQUOTED([$1], [$$3], [$4]);; esac rm -rf conftest*[]dnl ])# _AC_SYS_LARGEFILE_MACRO_VALUE # AC_SYS_LARGEFILE # ---------------- # By default, many hosts won't let programs access large files; # one must use special compiler options to get large-file access to work. # For more details about this brain damage please see: # http://www.unix-systems.org/version2/whatsnew/lfs20mar.html AC_DEFUN([AC_SYS_LARGEFILE], [AC_ARG_ENABLE(largefile, [ --disable-largefile omit support for large files]) if test "$enable_largefile" != no; then AC_CACHE_CHECK([for special C compiler options needed for large files], ac_cv_sys_largefile_CC, [ac_cv_sys_largefile_CC=no if test "$GCC" != yes; then ac_save_CC=$CC while :; do # IRIX 6.2 and later do not support large files by default, # so use the C compiler's -n32 option if that helps. AC_LANG_CONFTEST([AC_LANG_PROGRAM([_AC_SYS_LARGEFILE_TEST_INCLUDES])]) AC_COMPILE_IFELSE([], [break]) CC="$CC -n32" AC_COMPILE_IFELSE([], [ac_cv_sys_largefile_CC=' -n32'; break]) break done CC=$ac_save_CC rm -f conftest.$ac_ext fi]) if test "$ac_cv_sys_largefile_CC" != no; then CC=$CC$ac_cv_sys_largefile_CC fi _AC_SYS_LARGEFILE_MACRO_VALUE(_FILE_OFFSET_BITS, 64, ac_cv_sys_file_offset_bits, [Number of bits in a file offset, on hosts where this is settable.], [_AC_SYS_LARGEFILE_TEST_INCLUDES]) if test $ac_cv_sys_file_offset_bits = unknown; then _AC_SYS_LARGEFILE_MACRO_VALUE(_LARGE_FILES, 1, ac_cv_sys_large_files, [Define for large files, on AIX-style hosts.], [_AC_SYS_LARGEFILE_TEST_INCLUDES]) fi AC_DEFINE([_DARWIN_USE_64_BIT_INODE], [1], [Enable large inode numbers on Mac OS X 10.5.]) fi ])# AC_SYS_LARGEFILE ])# m4_version_prereq 2.70 # Enable large files on systems where this is implemented by Gnulib, not by the # system headers. # Set the variables WINDOWS_64_BIT_OFF_T, WINDOWS_64_BIT_ST_SIZE if Gnulib # overrides ensure that off_t or 'struct size.st_size' are 64-bit, respectively. AC_DEFUN([gl_LARGEFILE], [ AC_REQUIRE([AC_CANONICAL_HOST]) case "$host_os" in mingw*) dnl Native Windows. dnl mingw64 defines off_t to a 64-bit type already, if dnl _FILE_OFFSET_BITS=64, which is ensured by AC_SYS_LARGEFILE. AC_CACHE_CHECK([for 64-bit off_t], [gl_cv_type_off_t_64], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include int verify_off_t_size[sizeof (off_t) >= 8 ? 1 : -1]; ]], [[]])], [gl_cv_type_off_t_64=yes], [gl_cv_type_off_t_64=no]) ]) if test $gl_cv_type_off_t_64 = no; then WINDOWS_64_BIT_OFF_T=1 else WINDOWS_64_BIT_OFF_T=0 fi dnl But all native Windows platforms (including mingw64) have a 32-bit dnl st_size member in 'struct stat'. WINDOWS_64_BIT_ST_SIZE=1 ;; *) dnl Nothing to do on gnulib's side. dnl A 64-bit off_t is dnl - already the default on Mac OS X, FreeBSD, NetBSD, OpenBSD, IRIX, dnl OSF/1, Cygwin, dnl - enabled by _FILE_OFFSET_BITS=64 (ensured by AC_SYS_LARGEFILE) on dnl glibc, HP-UX, Solaris, dnl - enabled by _LARGE_FILES=1 (ensured by AC_SYS_LARGEFILE) on AIX, dnl - impossible to achieve on Minix 3.1.8. WINDOWS_64_BIT_OFF_T=0 WINDOWS_64_BIT_ST_SIZE=0 ;; esac ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/langinfo_h.m40000644000175000017500000000672113004436755016526 00000000000000# langinfo_h.m4 serial 7 dnl Copyright (C) 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_LANGINFO_H], [ AC_REQUIRE([gl_LANGINFO_H_DEFAULTS]) dnl Persuade glibc-2.0.6 to define CODESET. AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) dnl is always overridden, because of GNULIB_POSIXCHECK. gl_CHECK_NEXT_HEADERS([langinfo.h]) dnl Determine whether exists. It is missing on mingw and BeOS. HAVE_LANGINFO_CODESET=0 HAVE_LANGINFO_T_FMT_AMPM=0 HAVE_LANGINFO_ERA=0 HAVE_LANGINFO_YESEXPR=0 AC_CHECK_HEADERS_ONCE([langinfo.h]) if test $ac_cv_header_langinfo_h = yes; then HAVE_LANGINFO_H=1 dnl Determine what defines. CODESET and ERA etc. are missing dnl on OpenBSD 3.8. T_FMT_AMPM and YESEXPR, NOEXPR are missing on IRIX 5.3. AC_CACHE_CHECK([whether langinfo.h defines CODESET], [gl_cv_header_langinfo_codeset], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include int a = CODESET; ]])], [gl_cv_header_langinfo_codeset=yes], [gl_cv_header_langinfo_codeset=no]) ]) if test $gl_cv_header_langinfo_codeset = yes; then HAVE_LANGINFO_CODESET=1 fi AC_CACHE_CHECK([whether langinfo.h defines T_FMT_AMPM], [gl_cv_header_langinfo_t_fmt_ampm], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include int a = T_FMT_AMPM; ]])], [gl_cv_header_langinfo_t_fmt_ampm=yes], [gl_cv_header_langinfo_t_fmt_ampm=no]) ]) if test $gl_cv_header_langinfo_t_fmt_ampm = yes; then HAVE_LANGINFO_T_FMT_AMPM=1 fi AC_CACHE_CHECK([whether langinfo.h defines ERA], [gl_cv_header_langinfo_era], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include int a = ERA; ]])], [gl_cv_header_langinfo_era=yes], [gl_cv_header_langinfo_era=no]) ]) if test $gl_cv_header_langinfo_era = yes; then HAVE_LANGINFO_ERA=1 fi AC_CACHE_CHECK([whether langinfo.h defines YESEXPR], [gl_cv_header_langinfo_yesexpr], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include int a = YESEXPR; ]])], [gl_cv_header_langinfo_yesexpr=yes], [gl_cv_header_langinfo_yesexpr=no]) ]) if test $gl_cv_header_langinfo_yesexpr = yes; then HAVE_LANGINFO_YESEXPR=1 fi else HAVE_LANGINFO_H=0 fi AC_SUBST([HAVE_LANGINFO_H]) AC_SUBST([HAVE_LANGINFO_CODESET]) AC_SUBST([HAVE_LANGINFO_T_FMT_AMPM]) AC_SUBST([HAVE_LANGINFO_ERA]) AC_SUBST([HAVE_LANGINFO_YESEXPR]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[#include ]], [nl_langinfo]) ]) AC_DEFUN([gl_LANGINFO_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_LANGINFO_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_LANGINFO_H_DEFAULTS], [ GNULIB_NL_LANGINFO=0; AC_SUBST([GNULIB_NL_LANGINFO]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_NL_LANGINFO=1; AC_SUBST([HAVE_NL_LANGINFO]) REPLACE_NL_LANGINFO=0; AC_SUBST([REPLACE_NL_LANGINFO]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/inttypes_h.m40000644000175000017500000000177413004436755016613 00000000000000# inttypes_h.m4 serial 10 dnl Copyright (C) 1997-2004, 2006, 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Paul Eggert. # Define HAVE_INTTYPES_H_WITH_UINTMAX if exists, # doesn't clash with , and declares uintmax_t. AC_DEFUN([gl_AC_HEADER_INTTYPES_H], [ AC_CACHE_CHECK([for inttypes.h], [gl_cv_header_inttypes_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[ #include #include ]], [[uintmax_t i = (uintmax_t) -1; return !i;]])], [gl_cv_header_inttypes_h=yes], [gl_cv_header_inttypes_h=no])]) if test $gl_cv_header_inttypes_h = yes; then AC_DEFINE_UNQUOTED([HAVE_INTTYPES_H_WITH_UINTMAX], [1], [Define if exists, doesn't clash with , and declares uintmax_t. ]) fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/inttypes.m40000644000175000017500000001232013004436755016271 00000000000000# inttypes.m4 serial 26 dnl Copyright (C) 2006-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Derek Price, Bruno Haible. dnl Test whether is supported or must be substituted. AC_DEFUN([gl_INTTYPES_H], [ AC_REQUIRE([gl_INTTYPES_INCOMPLETE]) gl_INTTYPES_PRI_SCN ]) AC_DEFUN_ONCE([gl_INTTYPES_INCOMPLETE], [ AC_REQUIRE([gl_STDINT_H]) AC_CHECK_HEADERS_ONCE([inttypes.h]) dnl Override always, so that the portability warnings work. AC_REQUIRE([gl_INTTYPES_H_DEFAULTS]) gl_CHECK_NEXT_HEADERS([inttypes.h]) AC_REQUIRE([gl_MULTIARCH]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[#include ]], [imaxabs imaxdiv strtoimax strtoumax]) ]) # Ensure that the PRI* and SCN* macros are defined appropriately. AC_DEFUN([gl_INTTYPES_PRI_SCN], [ AC_REQUIRE([gt_INTTYPES_PRI]) PRIPTR_PREFIX= if test -n "$STDINT_H"; then dnl Using the gnulib . It always defines intptr_t to 'long'. PRIPTR_PREFIX='"l"' else dnl Using the system's . for glpfx in '' l ll I64; do case $glpfx in '') gltype1='int';; l) gltype1='long int';; ll) gltype1='long long int';; I64) gltype1='__int64';; esac AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include extern intptr_t foo; extern $gltype1 foo;]])], [PRIPTR_PREFIX='"'$glpfx'"']) test -n "$PRIPTR_PREFIX" && break done fi AC_SUBST([PRIPTR_PREFIX]) gl_INTTYPES_CHECK_LONG_LONG_INT_CONDITION( [INT32_MAX_LT_INTMAX_MAX], [defined INT32_MAX && defined INTMAX_MAX], [INT32_MAX < INTMAX_MAX], [sizeof (int) < sizeof (long long int)]) if test $APPLE_UNIVERSAL_BUILD = 0; then gl_INTTYPES_CHECK_LONG_LONG_INT_CONDITION( [INT64_MAX_EQ_LONG_MAX], [defined INT64_MAX], [INT64_MAX == LONG_MAX], [sizeof (long long int) == sizeof (long int)]) else INT64_MAX_EQ_LONG_MAX=-1 fi gl_INTTYPES_CHECK_LONG_LONG_INT_CONDITION( [UINT32_MAX_LT_UINTMAX_MAX], [defined UINT32_MAX && defined UINTMAX_MAX], [UINT32_MAX < UINTMAX_MAX], [sizeof (unsigned int) < sizeof (unsigned long long int)]) if test $APPLE_UNIVERSAL_BUILD = 0; then gl_INTTYPES_CHECK_LONG_LONG_INT_CONDITION( [UINT64_MAX_EQ_ULONG_MAX], [defined UINT64_MAX], [UINT64_MAX == ULONG_MAX], [sizeof (unsigned long long int) == sizeof (unsigned long int)]) else UINT64_MAX_EQ_ULONG_MAX=-1 fi ]) # Define the symbol $1 to be 1 if the condition is true, 0 otherwise. # If $2 is true, the condition is $3; otherwise if long long int is supported # approximate the condition with $4; otherwise, assume the condition is false. # The condition should work on all C99 platforms; the approximations should be # good enough to work on all practical pre-C99 platforms. # $2 is evaluated by the C preprocessor, $3 and $4 as compile-time constants. AC_DEFUN([gl_INTTYPES_CHECK_LONG_LONG_INT_CONDITION], [ AC_CACHE_CHECK([whether $3], [gl_cv_test_$1], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[/* Work also in C++ mode. */ #define __STDC_LIMIT_MACROS 1 /* Work if build is not clean. */ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H #include #if HAVE_STDINT_H #include #endif #if $2 #define CONDITION ($3) #elif HAVE_LONG_LONG_INT #define CONDITION ($4) #else #define CONDITION 0 #endif int test[CONDITION ? 1 : -1];]])], [gl_cv_test_$1=yes], [gl_cv_test_$1=no])]) if test $gl_cv_test_$1 = yes; then $1=1; else $1=0; fi AC_SUBST([$1]) ]) AC_DEFUN([gl_INTTYPES_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_INTTYPES_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) ]) AC_DEFUN([gl_INTTYPES_H_DEFAULTS], [ GNULIB_IMAXABS=0; AC_SUBST([GNULIB_IMAXABS]) GNULIB_IMAXDIV=0; AC_SUBST([GNULIB_IMAXDIV]) GNULIB_STRTOIMAX=0; AC_SUBST([GNULIB_STRTOIMAX]) GNULIB_STRTOUMAX=0; AC_SUBST([GNULIB_STRTOUMAX]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_DECL_IMAXABS=1; AC_SUBST([HAVE_DECL_IMAXABS]) HAVE_DECL_IMAXDIV=1; AC_SUBST([HAVE_DECL_IMAXDIV]) HAVE_DECL_STRTOIMAX=1; AC_SUBST([HAVE_DECL_STRTOIMAX]) HAVE_DECL_STRTOUMAX=1; AC_SUBST([HAVE_DECL_STRTOUMAX]) REPLACE_STRTOIMAX=0; AC_SUBST([REPLACE_STRTOIMAX]) REPLACE_STRTOUMAX=0; AC_SUBST([REPLACE_STRTOUMAX]) INT32_MAX_LT_INTMAX_MAX=1; AC_SUBST([INT32_MAX_LT_INTMAX_MAX]) INT64_MAX_EQ_LONG_MAX='defined _LP64'; AC_SUBST([INT64_MAX_EQ_LONG_MAX]) PRI_MACROS_BROKEN=0; AC_SUBST([PRI_MACROS_BROKEN]) PRIPTR_PREFIX=__PRIPTR_PREFIX; AC_SUBST([PRIPTR_PREFIX]) UINT32_MAX_LT_UINTMAX_MAX=1; AC_SUBST([UINT32_MAX_LT_UINTMAX_MAX]) UINT64_MAX_EQ_ULONG_MAX='defined _LP64'; AC_SUBST([UINT64_MAX_EQ_ULONG_MAX]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/inttypes-pri.m40000644000175000017500000000234513004436755017067 00000000000000# inttypes-pri.m4 serial 7 (gettext-0.18.2) dnl Copyright (C) 1997-2002, 2006, 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. AC_PREREQ([2.53]) # Define PRI_MACROS_BROKEN if exists and defines the PRI* # macros to non-string values. This is the case on AIX 4.3.3. AC_DEFUN([gt_INTTYPES_PRI], [ AC_CHECK_HEADERS([inttypes.h]) if test $ac_cv_header_inttypes_h = yes; then AC_CACHE_CHECK([whether the inttypes.h PRIxNN macros are broken], [gt_cv_inttypes_pri_broken], [ AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[ #include #ifdef PRId32 char *p = PRId32; #endif ]], [[]])], [gt_cv_inttypes_pri_broken=no], [gt_cv_inttypes_pri_broken=yes]) ]) fi if test "$gt_cv_inttypes_pri_broken" = yes; then AC_DEFINE_UNQUOTED([PRI_MACROS_BROKEN], [1], [Define if exists and defines unusable PRI* macros.]) PRI_MACROS_BROKEN=1 else PRI_MACROS_BROKEN=0 fi AC_SUBST([PRI_MACROS_BROKEN]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/intmax_t.m40000644000175000017500000000416613004436755016246 00000000000000# intmax_t.m4 serial 8 dnl Copyright (C) 1997-2004, 2006-2007, 2009-2016 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Paul Eggert. AC_PREREQ([2.53]) # Define intmax_t to 'long' or 'long long' # if it is not already defined in or . AC_DEFUN([gl_AC_TYPE_INTMAX_T], [ dnl For simplicity, we assume that a header file defines 'intmax_t' if and dnl only if it defines 'uintmax_t'. AC_REQUIRE([gl_AC_HEADER_INTTYPES_H]) AC_REQUIRE([gl_AC_HEADER_STDINT_H]) if test $gl_cv_header_inttypes_h = no && test $gl_cv_header_stdint_h = no; then AC_REQUIRE([AC_TYPE_LONG_LONG_INT]) test $ac_cv_type_long_long_int = yes \ && ac_type='long long' \ || ac_type='long' AC_DEFINE_UNQUOTED([intmax_t], [$ac_type], [Define to long or long long if and don't define.]) else AC_DEFINE([HAVE_INTMAX_T], [1], [Define if you have the 'intmax_t' type in or .]) fi ]) dnl An alternative would be to explicitly test for 'intmax_t'. AC_DEFUN([gt_AC_TYPE_INTMAX_T], [ AC_REQUIRE([gl_AC_HEADER_INTTYPES_H]) AC_REQUIRE([gl_AC_HEADER_STDINT_H]) AC_CACHE_CHECK([for intmax_t], [gt_cv_c_intmax_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[ #include #include #if HAVE_STDINT_H_WITH_UINTMAX #include #endif #if HAVE_INTTYPES_H_WITH_UINTMAX #include #endif ]], [[intmax_t x = -1; return !x;]])], [gt_cv_c_intmax_t=yes], [gt_cv_c_intmax_t=no])]) if test $gt_cv_c_intmax_t = yes; then AC_DEFINE([HAVE_INTMAX_T], [1], [Define if you have the 'intmax_t' type in or .]) else AC_REQUIRE([AC_TYPE_LONG_LONG_INT]) test $ac_cv_type_long_long_int = yes \ && ac_type='long long' \ || ac_type='long' AC_DEFINE_UNQUOTED([intmax_t], [$ac_type], [Define to long or long long if and don't define.]) fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/intlmacosx.m40000644000175000017500000000474513004436755016607 00000000000000# intlmacosx.m4 serial 5 (gettext-0.18.2) dnl Copyright (C) 2004-2014, 2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl dnl This file can be used in projects which are not available under dnl the GNU General Public License or the GNU Library General Public dnl License but which still want to provide support for the GNU gettext dnl functionality. dnl Please note that the actual code of the GNU gettext library is covered dnl by the GNU Library General Public License, and the rest of the GNU dnl gettext package is covered by the GNU General Public License. dnl They are *not* in the public domain. dnl Checks for special options needed on Mac OS X. dnl Defines INTL_MACOSX_LIBS. AC_DEFUN([gt_INTL_MACOSX], [ dnl Check for API introduced in Mac OS X 10.2. AC_CACHE_CHECK([for CFPreferencesCopyAppValue], [gt_cv_func_CFPreferencesCopyAppValue], [gt_save_LIBS="$LIBS" LIBS="$LIBS -Wl,-framework -Wl,CoreFoundation" AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[CFPreferencesCopyAppValue(NULL, NULL)]])], [gt_cv_func_CFPreferencesCopyAppValue=yes], [gt_cv_func_CFPreferencesCopyAppValue=no]) LIBS="$gt_save_LIBS"]) if test $gt_cv_func_CFPreferencesCopyAppValue = yes; then AC_DEFINE([HAVE_CFPREFERENCESCOPYAPPVALUE], [1], [Define to 1 if you have the Mac OS X function CFPreferencesCopyAppValue in the CoreFoundation framework.]) fi dnl Check for API introduced in Mac OS X 10.3. AC_CACHE_CHECK([for CFLocaleCopyCurrent], [gt_cv_func_CFLocaleCopyCurrent], [gt_save_LIBS="$LIBS" LIBS="$LIBS -Wl,-framework -Wl,CoreFoundation" AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[CFLocaleCopyCurrent();]])], [gt_cv_func_CFLocaleCopyCurrent=yes], [gt_cv_func_CFLocaleCopyCurrent=no]) LIBS="$gt_save_LIBS"]) if test $gt_cv_func_CFLocaleCopyCurrent = yes; then AC_DEFINE([HAVE_CFLOCALECOPYCURRENT], [1], [Define to 1 if you have the Mac OS X function CFLocaleCopyCurrent in the CoreFoundation framework.]) fi INTL_MACOSX_LIBS= if test $gt_cv_func_CFPreferencesCopyAppValue = yes || test $gt_cv_func_CFLocaleCopyCurrent = yes; then INTL_MACOSX_LIBS="-Wl,-framework -Wl,CoreFoundation" fi AC_SUBST([INTL_MACOSX_LIBS]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/include_next.m40000644000175000017500000002077313004436755017106 00000000000000# include_next.m4 serial 23 dnl Copyright (C) 2006-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Paul Eggert and Derek Price. dnl Sets INCLUDE_NEXT and PRAGMA_SYSTEM_HEADER. dnl dnl INCLUDE_NEXT expands to 'include_next' if the compiler supports it, or to dnl 'include' otherwise. dnl dnl INCLUDE_NEXT_AS_FIRST_DIRECTIVE expands to 'include_next' if the compiler dnl supports it in the special case that it is the first include directive in dnl the given file, or to 'include' otherwise. dnl dnl PRAGMA_SYSTEM_HEADER can be used in files that contain #include_next, dnl so as to avoid GCC warnings when the gcc option -pedantic is used. dnl '#pragma GCC system_header' has the same effect as if the file was found dnl through the include search path specified with '-isystem' options (as dnl opposed to the search path specified with '-I' options). Namely, gcc dnl does not warn about some things, and on some systems (Solaris and Interix) dnl __STDC__ evaluates to 0 instead of to 1. The latter is an undesired side dnl effect; we are therefore careful to use 'defined __STDC__' or '1' instead dnl of plain '__STDC__'. dnl dnl PRAGMA_COLUMNS can be used in files that override system header files, so dnl as to avoid compilation errors on HP NonStop systems when the gnulib file dnl is included by a system header file that does a "#pragma COLUMNS 80" (which dnl has the effect of truncating the lines of that file and all files that it dnl includes to 80 columns) and the gnulib file has lines longer than 80 dnl columns. AC_DEFUN([gl_INCLUDE_NEXT], [ AC_LANG_PREPROC_REQUIRE() AC_CACHE_CHECK([whether the preprocessor supports include_next], [gl_cv_have_include_next], [rm -rf conftestd1a conftestd1b conftestd2 mkdir conftestd1a conftestd1b conftestd2 dnl IBM C 9.0, 10.1 (original versions, prior to the 2009-01 updates) on dnl AIX 6.1 support include_next when used as first preprocessor directive dnl in a file, but not when preceded by another include directive. Check dnl for this bug by including . dnl Additionally, with this same compiler, include_next is a no-op when dnl used in a header file that was included by specifying its absolute dnl file name. Despite these two bugs, include_next is used in the dnl compiler's . By virtue of the second bug, we need to use dnl include_next as well in this case. cat < conftestd1a/conftest.h #define DEFINED_IN_CONFTESTD1 #include_next #ifdef DEFINED_IN_CONFTESTD2 int foo; #else #error "include_next doesn't work" #endif EOF cat < conftestd1b/conftest.h #define DEFINED_IN_CONFTESTD1 #include #include_next #ifdef DEFINED_IN_CONFTESTD2 int foo; #else #error "include_next doesn't work" #endif EOF cat < conftestd2/conftest.h #ifndef DEFINED_IN_CONFTESTD1 #error "include_next test doesn't work" #endif #define DEFINED_IN_CONFTESTD2 EOF gl_save_CPPFLAGS="$CPPFLAGS" CPPFLAGS="$gl_save_CPPFLAGS -Iconftestd1b -Iconftestd2" dnl We intentionally avoid using AC_LANG_SOURCE here. AC_COMPILE_IFELSE([AC_LANG_DEFINES_PROVIDED[#include ]], [gl_cv_have_include_next=yes], [CPPFLAGS="$gl_save_CPPFLAGS -Iconftestd1a -Iconftestd2" AC_COMPILE_IFELSE([AC_LANG_DEFINES_PROVIDED[#include ]], [gl_cv_have_include_next=buggy], [gl_cv_have_include_next=no]) ]) CPPFLAGS="$gl_save_CPPFLAGS" rm -rf conftestd1a conftestd1b conftestd2 ]) PRAGMA_SYSTEM_HEADER= if test $gl_cv_have_include_next = yes; then INCLUDE_NEXT=include_next INCLUDE_NEXT_AS_FIRST_DIRECTIVE=include_next if test -n "$GCC"; then PRAGMA_SYSTEM_HEADER='#pragma GCC system_header' fi else if test $gl_cv_have_include_next = buggy; then INCLUDE_NEXT=include INCLUDE_NEXT_AS_FIRST_DIRECTIVE=include_next else INCLUDE_NEXT=include INCLUDE_NEXT_AS_FIRST_DIRECTIVE=include fi fi AC_SUBST([INCLUDE_NEXT]) AC_SUBST([INCLUDE_NEXT_AS_FIRST_DIRECTIVE]) AC_SUBST([PRAGMA_SYSTEM_HEADER]) AC_CACHE_CHECK([whether system header files limit the line length], [gl_cv_pragma_columns], [dnl HP NonStop systems, which define __TANDEM, have this misfeature. AC_EGREP_CPP([choke me], [ #ifdef __TANDEM choke me #endif ], [gl_cv_pragma_columns=yes], [gl_cv_pragma_columns=no]) ]) if test $gl_cv_pragma_columns = yes; then PRAGMA_COLUMNS="#pragma COLUMNS 10000" else PRAGMA_COLUMNS= fi AC_SUBST([PRAGMA_COLUMNS]) ]) # gl_CHECK_NEXT_HEADERS(HEADER1 HEADER2 ...) # ------------------------------------------ # For each arg foo.h, if #include_next works, define NEXT_FOO_H to be # ''; otherwise define it to be # '"///usr/include/foo.h"', or whatever other absolute file name is suitable. # Also, if #include_next works as first preprocessing directive in a file, # define NEXT_AS_FIRST_DIRECTIVE_FOO_H to be ''; otherwise define it to # be # '"///usr/include/foo.h"', or whatever other absolute file name is suitable. # That way, a header file with the following line: # #@INCLUDE_NEXT@ @NEXT_FOO_H@ # or # #@INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ @NEXT_AS_FIRST_DIRECTIVE_FOO_H@ # behaves (after sed substitution) as if it contained # #include_next # even if the compiler does not support include_next. # The three "///" are to pacify Sun C 5.8, which otherwise would say # "warning: #include of /usr/include/... may be non-portable". # Use '""', not '<>', so that the /// cannot be confused with a C99 comment. # Note: This macro assumes that the header file is not empty after # preprocessing, i.e. it does not only define preprocessor macros but also # provides some type/enum definitions or function/variable declarations. # # This macro also checks whether each header exists, by invoking # AC_CHECK_HEADERS_ONCE or AC_CHECK_HEADERS on each argument. AC_DEFUN([gl_CHECK_NEXT_HEADERS], [ gl_NEXT_HEADERS_INTERNAL([$1], [check]) ]) # gl_NEXT_HEADERS(HEADER1 HEADER2 ...) # ------------------------------------ # Like gl_CHECK_NEXT_HEADERS, except do not check whether the headers exist. # This is suitable for headers like that are standardized by C89 # and therefore can be assumed to exist. AC_DEFUN([gl_NEXT_HEADERS], [ gl_NEXT_HEADERS_INTERNAL([$1], [assume]) ]) # The guts of gl_CHECK_NEXT_HEADERS and gl_NEXT_HEADERS. AC_DEFUN([gl_NEXT_HEADERS_INTERNAL], [ AC_REQUIRE([gl_INCLUDE_NEXT]) AC_REQUIRE([AC_CANONICAL_HOST]) m4_if([$2], [check], [AC_CHECK_HEADERS_ONCE([$1]) ]) dnl FIXME: gl_next_header and gl_header_exists must be used unquoted dnl until we can assume autoconf 2.64 or newer. m4_foreach_w([gl_HEADER_NAME], [$1], [AS_VAR_PUSHDEF([gl_next_header], [gl_cv_next_]m4_defn([gl_HEADER_NAME])) if test $gl_cv_have_include_next = yes; then AS_VAR_SET(gl_next_header, ['<'gl_HEADER_NAME'>']) else AC_CACHE_CHECK( [absolute name of <]m4_defn([gl_HEADER_NAME])[>], m4_defn([gl_next_header]), [m4_if([$2], [check], [AS_VAR_PUSHDEF([gl_header_exists], [ac_cv_header_]m4_defn([gl_HEADER_NAME])) if test AS_VAR_GET(gl_header_exists) = yes; then AS_VAR_POPDEF([gl_header_exists]) ]) gl_ABSOLUTE_HEADER_ONE(gl_HEADER_NAME) AS_VAR_COPY([gl_header], [gl_cv_absolute_]AS_TR_SH(gl_HEADER_NAME)) AS_VAR_SET(gl_next_header, ['"'$gl_header'"']) m4_if([$2], [check], [else AS_VAR_SET(gl_next_header, ['<'gl_HEADER_NAME'>']) fi ]) ]) fi AC_SUBST( AS_TR_CPP([NEXT_]m4_defn([gl_HEADER_NAME])), [AS_VAR_GET(gl_next_header)]) if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'gl_HEADER_NAME'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=AS_VAR_GET(gl_next_header) fi AC_SUBST( AS_TR_CPP([NEXT_AS_FIRST_DIRECTIVE_]m4_defn([gl_HEADER_NAME])), [$gl_next_as_first_directive]) AS_VAR_POPDEF([gl_next_header])]) ]) # Autoconf 2.68 added warnings for our use of AC_COMPILE_IFELSE; # this fallback is safe for all earlier autoconf versions. m4_define_default([AC_LANG_DEFINES_PROVIDED]) gnuastro-0.2.33-8a3b/bootstrapped/m4/hard-locale.m40000644000175000017500000000056213004436755016572 00000000000000# hard-locale.m4 serial 8 dnl Copyright (C) 2002-2006, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl No prerequisites of lib/hard-locale.c. AC_DEFUN([gl_HARD_LOCALE], [ : ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/gnulib-comp.m40000644000175000017500000007667413004436762016652 00000000000000# DO NOT EDIT! GENERATED AUTOMATICALLY! # Copyright (C) 2002-2016 Free Software Foundation, Inc. # # This file is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This file is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this file. If not, see . # # As a special exception to the GNU General Public License, # this file may be distributed as part of a program that # contains a configuration script generated by Autoconf, under # the same distribution terms as the rest of that program. # # Generated by gnulib-tool. # # This file represents the compiled summary of the specification in # gnulib-cache.m4. It lists the computed macro invocations that need # to be invoked from configure.ac. # In projects that use version control, this file can be treated like # other built files. # This macro should be invoked from ./configure.ac, in the section # "Checks for programs", right after AC_PROG_CC, and certainly before # any checks for libraries, header files, types and library functions. AC_DEFUN([gl_EARLY], [ m4_pattern_forbid([^gl_[A-Z]])dnl the gnulib macro namespace m4_pattern_allow([^gl_ES$])dnl a valid locale name m4_pattern_allow([^gl_LIBOBJS$])dnl a variable m4_pattern_allow([^gl_LTLIBOBJS$])dnl a variable # Pre-early section. AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([gl_PROG_AR_RANLIB]) AC_REQUIRE([AM_PROG_CC_C_O]) # Code from module absolute-header: # Code from module alloca: # Code from module alloca-opt: # Code from module alloca-opt-tests: # Code from module argp: # Code from module argp-tests: # Code from module binary-io: # Code from module binary-io-tests: # Code from module btowc: # Code from module btowc-tests: # Code from module c-ctype: # Code from module c-ctype-tests: # Code from module c-strcase: # Code from module c-strcase-tests: # Code from module close: # Code from module close-tests: # Code from module configmake: # Code from module ctype: # Code from module ctype-tests: # Code from module dirname-lgpl: # Code from module dosname: # Code from module double-slash-root: # Code from module dup2: # Code from module dup2-tests: # Code from module environ: # Code from module environ-tests: # Code from module errno: # Code from module errno-tests: # Code from module error: # Code from module extensions: # Code from module extern-inline: # Code from module fcntl-h: # Code from module fcntl-h-tests: # Code from module fd-hook: # Code from module fdl: # Code from module fdopen: # Code from module fdopen-tests: # Code from module fgetc-tests: # Code from module flexmember: # Code from module float: # Code from module float-tests: # Code from module fpieee: AC_REQUIRE([gl_FP_IEEE]) # Code from module fpucw: # Code from module fputc-tests: # Code from module fread-tests: # Code from module fstat: # Code from module fstat-tests: # Code from module fwrite-tests: # Code from module gendocs: # Code from module getcwd-lgpl: # Code from module getcwd-lgpl-tests: # Code from module getdtablesize: # Code from module getdtablesize-tests: # Code from module getopt-gnu: # Code from module getopt-posix: # Code from module getopt-posix-tests: # Code from module getpagesize: # Code from module getprogname: # Code from module getprogname-tests: # Code from module gettext-h: # Code from module gettimeofday: # Code from module gettimeofday-tests: # Code from module git-version-gen: # Code from module hard-locale: # Code from module havelib: # Code from module ignore-value: # Code from module ignore-value-tests: # Code from module include_next: # Code from module intprops: # Code from module intprops-tests: # Code from module inttypes: # Code from module inttypes-incomplete: # Code from module inttypes-tests: # Code from module langinfo: # Code from module langinfo-tests: # Code from module largefile: AC_REQUIRE([AC_SYS_LARGEFILE]) # Code from module limits-h: # Code from module limits-h-tests: # Code from module localcharset: # Code from module locale: # Code from module locale-tests: # Code from module localeconv: # Code from module localeconv-tests: # Code from module localename: # Code from module localename-tests: # Code from module lock: # Code from module lock-tests: # Code from module lstat: # Code from module lstat-tests: # Code from module malloc-gnu: # Code from module malloc-gnu-tests: # Code from module malloc-posix: # Code from module malloca: # Code from module malloca-tests: # Code from module math: # Code from module math-tests: # Code from module mbrtowc: # Code from module mbrtowc-tests: # Code from module mbsinit: # Code from module mbsinit-tests: # Code from module mbtowc: # Code from module memchr: # Code from module memchr-tests: # Code from module mempcpy: # Code from module msvc-inval: # Code from module msvc-nothrow: # Code from module multiarch: # Code from module nl_langinfo: # Code from module nl_langinfo-tests: # Code from module nocrash: # Code from module nproc: # Code from module open: # Code from module open-tests: # Code from module pathmax: # Code from module pathmax-tests: # Code from module putenv: # Code from module rawmemchr: # Code from module rawmemchr-tests: # Code from module regex: # Code from module regex-tests: # Code from module same-inode: # Code from module setenv: # Code from module setenv-tests: # Code from module setlocale: # Code from module setlocale-tests: # Code from module size_max: # Code from module sleep: # Code from module sleep-tests: # Code from module snippet/_Noreturn: # Code from module snippet/arg-nonnull: # Code from module snippet/c++defs: # Code from module snippet/warn-on-use: # Code from module ssize_t: # Code from module stat: # Code from module stat-tests: # Code from module stdalign: # Code from module stdalign-tests: # Code from module stdbool: # Code from module stdbool-tests: # Code from module stddef: # Code from module stddef-tests: # Code from module stdint: # Code from module stdint-tests: # Code from module stdio: # Code from module stdio-tests: # Code from module stdlib: # Code from module stdlib-tests: # Code from module strcase: # Code from module strchrnul: # Code from module strchrnul-tests: # Code from module streq: # Code from module strerror: # Code from module strerror-override: # Code from module strerror-tests: # Code from module string: # Code from module string-tests: # Code from module strings: # Code from module strings-tests: # Code from module strndup: # Code from module strnlen: # Code from module strnlen-tests: # Code from module symlink: # Code from module symlink-tests: # Code from module sys_stat: # Code from module sys_stat-tests: # Code from module sys_time: # Code from module sys_time-tests: # Code from module sys_types: # Code from module sys_types-tests: # Code from module sysexits: # Code from module sysexits-tests: # Code from module test-framework-sh: # Code from module test-framework-sh-tests: # Code from module thread: # Code from module thread-tests: # Code from module threadlib: gl_THREADLIB_EARLY # Code from module time: # Code from module time-tests: # Code from module unistd: # Code from module unistd-tests: # Code from module unsetenv: # Code from module unsetenv-tests: # Code from module vasnprintf: # Code from module vasnprintf-tests: # Code from module verify: # Code from module verify-tests: # Code from module vsnprintf: # Code from module vsnprintf-tests: # Code from module wchar: # Code from module wchar-tests: # Code from module wcrtomb: # Code from module wcrtomb-tests: # Code from module wctob: # Code from module wctomb: # Code from module wctype-h: # Code from module wctype-h-tests: # Code from module xsize: # Code from module yield: ]) # This macro should be invoked from ./configure.ac, in the section # "Check for header files, types and library functions". AC_DEFUN([gl_INIT], [ AM_CONDITIONAL([GL_COND_LIBTOOL], [true]) gl_cond_libtool=true gl_m4_base='bootstrapped/m4' m4_pushdef([AC_LIBOBJ], m4_defn([gl_LIBOBJ])) m4_pushdef([AC_REPLACE_FUNCS], m4_defn([gl_REPLACE_FUNCS])) m4_pushdef([AC_LIBSOURCES], m4_defn([gl_LIBSOURCES])) m4_pushdef([gl_LIBSOURCES_LIST], []) m4_pushdef([gl_LIBSOURCES_DIR], []) gl_COMMON gl_source_base='bootstrapped/lib' changequote(,)dnl LTALLOCA=`echo "$ALLOCA" | sed -e 's/\.[^.]* /.lo /g;s/\.[^.]*$/.lo/'` changequote([, ])dnl AC_SUBST([LTALLOCA]) gl_FUNC_ALLOCA gl_ARGP m4_ifdef([AM_XGETTEXT_OPTION], [AM_][XGETTEXT_OPTION([--flag=argp_error:2:c-format]) AM_][XGETTEXT_OPTION([--flag=argp_failure:4:c-format])]) gl_FUNC_BTOWC if test $HAVE_BTOWC = 0 || test $REPLACE_BTOWC = 1; then AC_LIBOBJ([btowc]) gl_PREREQ_BTOWC fi gl_WCHAR_MODULE_INDICATOR([btowc]) gl_CONFIGMAKE_PREP gl_DIRNAME_LGPL gl_DOUBLE_SLASH_ROOT gl_HEADER_ERRNO_H gl_ERROR if test $ac_cv_lib_error_at_line = no; then AC_LIBOBJ([error]) gl_PREREQ_ERROR fi m4_ifdef([AM_XGETTEXT_OPTION], [AM_][XGETTEXT_OPTION([--flag=error:3:c-format]) AM_][XGETTEXT_OPTION([--flag=error_at_line:5:c-format])]) AC_REQUIRE([gl_EXTERN_INLINE]) gl_FLOAT_H if test $REPLACE_FLOAT_LDBL = 1; then AC_LIBOBJ([float]) fi if test $REPLACE_ITOLD = 1; then AC_LIBOBJ([itold]) fi gl_FUNC_GETOPT_GNU if test $REPLACE_GETOPT = 1; then AC_LIBOBJ([getopt]) AC_LIBOBJ([getopt1]) gl_PREREQ_GETOPT dnl Arrange for unistd.h to include getopt.h. GNULIB_GL_UNISTD_H_GETOPT=1 fi AC_SUBST([GNULIB_GL_UNISTD_H_GETOPT]) gl_MODULE_INDICATOR_FOR_TESTS([getopt-gnu]) gl_FUNC_GETOPT_POSIX if test $REPLACE_GETOPT = 1; then AC_LIBOBJ([getopt]) AC_LIBOBJ([getopt1]) gl_PREREQ_GETOPT dnl Arrange for unistd.h to include getopt.h. GNULIB_GL_UNISTD_H_GETOPT=1 fi AC_SUBST([GNULIB_GL_UNISTD_H_GETOPT]) gl_FUNC_GETPROGNAME AC_SUBST([LIBINTL]) AC_SUBST([LTLIBINTL]) gl_HARD_LOCALE gl_LANGINFO_H gl_LIMITS_H gl_LOCALCHARSET LOCALCHARSET_TESTS_ENVIRONMENT="CHARSETALIASDIR=\"\$(abs_top_builddir)/$gl_source_base\"" AC_SUBST([LOCALCHARSET_TESTS_ENVIRONMENT]) gl_LOCALE_H gl_FUNC_LOCALECONV if test $REPLACE_LOCALECONV = 1; then AC_LIBOBJ([localeconv]) gl_PREREQ_LOCALECONV fi gl_LOCALE_MODULE_INDICATOR([localeconv]) gl_LOCK gl_MODULE_INDICATOR([lock]) gl_FUNC_MALLOC_GNU if test $REPLACE_MALLOC = 1; then AC_LIBOBJ([malloc]) fi gl_MODULE_INDICATOR([malloc-gnu]) gl_FUNC_MALLOC_POSIX if test $REPLACE_MALLOC = 1; then AC_LIBOBJ([malloc]) fi gl_STDLIB_MODULE_INDICATOR([malloc-posix]) gl_MATH_H gl_FUNC_MBRTOWC if test $HAVE_MBRTOWC = 0 || test $REPLACE_MBRTOWC = 1; then AC_LIBOBJ([mbrtowc]) gl_PREREQ_MBRTOWC fi gl_WCHAR_MODULE_INDICATOR([mbrtowc]) gl_FUNC_MBSINIT if test $HAVE_MBSINIT = 0 || test $REPLACE_MBSINIT = 1; then AC_LIBOBJ([mbsinit]) gl_PREREQ_MBSINIT fi gl_WCHAR_MODULE_INDICATOR([mbsinit]) gl_FUNC_MBTOWC if test $REPLACE_MBTOWC = 1; then AC_LIBOBJ([mbtowc]) gl_PREREQ_MBTOWC fi gl_STDLIB_MODULE_INDICATOR([mbtowc]) gl_FUNC_MEMCHR if test $HAVE_MEMCHR = 0 || test $REPLACE_MEMCHR = 1; then AC_LIBOBJ([memchr]) gl_PREREQ_MEMCHR fi gl_STRING_MODULE_INDICATOR([memchr]) gl_FUNC_MEMPCPY if test $HAVE_MEMPCPY = 0; then AC_LIBOBJ([mempcpy]) gl_PREREQ_MEMPCPY fi gl_STRING_MODULE_INDICATOR([mempcpy]) AC_REQUIRE([gl_MSVC_INVAL]) if test $HAVE_MSVC_INVALID_PARAMETER_HANDLER = 1; then AC_LIBOBJ([msvc-inval]) fi AC_REQUIRE([gl_MSVC_NOTHROW]) if test $HAVE_MSVC_INVALID_PARAMETER_HANDLER = 1; then AC_LIBOBJ([msvc-nothrow]) fi gl_MULTIARCH gl_FUNC_NL_LANGINFO if test $HAVE_NL_LANGINFO = 0 || test $REPLACE_NL_LANGINFO = 1; then AC_LIBOBJ([nl_langinfo]) fi gl_LANGINFO_MODULE_INDICATOR([nl_langinfo]) gl_NPROC gl_FUNC_RAWMEMCHR if test $HAVE_RAWMEMCHR = 0; then AC_LIBOBJ([rawmemchr]) gl_PREREQ_RAWMEMCHR fi gl_STRING_MODULE_INDICATOR([rawmemchr]) gl_REGEX if test $ac_use_included_regex = yes; then AC_LIBOBJ([regex]) gl_PREREQ_REGEX fi gl_SIZE_MAX gl_FUNC_SLEEP if test $HAVE_SLEEP = 0 || test $REPLACE_SLEEP = 1; then AC_LIBOBJ([sleep]) fi gl_UNISTD_MODULE_INDICATOR([sleep]) gt_TYPE_SSIZE_T gl_STDALIGN_H AM_STDBOOL_H gl_STDDEF_H gl_STDINT_H gl_STDIO_H gl_STDLIB_H gl_STRCASE if test $HAVE_STRCASECMP = 0; then AC_LIBOBJ([strcasecmp]) gl_PREREQ_STRCASECMP fi if test $HAVE_STRNCASECMP = 0; then AC_LIBOBJ([strncasecmp]) gl_PREREQ_STRNCASECMP fi gl_FUNC_STRCHRNUL if test $HAVE_STRCHRNUL = 0 || test $REPLACE_STRCHRNUL = 1; then AC_LIBOBJ([strchrnul]) gl_PREREQ_STRCHRNUL fi gl_STRING_MODULE_INDICATOR([strchrnul]) gl_FUNC_STRERROR if test $REPLACE_STRERROR = 1; then AC_LIBOBJ([strerror]) fi gl_MODULE_INDICATOR([strerror]) gl_STRING_MODULE_INDICATOR([strerror]) AC_REQUIRE([gl_HEADER_ERRNO_H]) AC_REQUIRE([gl_FUNC_STRERROR_0]) if test -n "$ERRNO_H" || test $REPLACE_STRERROR_0 = 1; then AC_LIBOBJ([strerror-override]) gl_PREREQ_SYS_H_WINSOCK2 fi gl_HEADER_STRING_H gl_HEADER_STRINGS_H gl_FUNC_STRNDUP if test $HAVE_STRNDUP = 0 || test $REPLACE_STRNDUP = 1; then AC_LIBOBJ([strndup]) fi gl_STRING_MODULE_INDICATOR([strndup]) gl_FUNC_STRNLEN if test $HAVE_DECL_STRNLEN = 0 || test $REPLACE_STRNLEN = 1; then AC_LIBOBJ([strnlen]) gl_PREREQ_STRNLEN fi gl_STRING_MODULE_INDICATOR([strnlen]) gl_SYS_TYPES_H AC_PROG_MKDIR_P gl_SYSEXITS gl_THREADLIB gl_UNISTD_H gl_FUNC_VASNPRINTF gl_FUNC_VSNPRINTF gl_STDIO_MODULE_INDICATOR([vsnprintf]) gl_WCHAR_H gl_FUNC_WCRTOMB if test $HAVE_WCRTOMB = 0 || test $REPLACE_WCRTOMB = 1; then AC_LIBOBJ([wcrtomb]) gl_PREREQ_WCRTOMB fi gl_WCHAR_MODULE_INDICATOR([wcrtomb]) gl_WCTYPE_H gl_XSIZE # End of code from modules m4_ifval(gl_LIBSOURCES_LIST, [ m4_syscmd([test ! -d ]m4_defn([gl_LIBSOURCES_DIR])[ || for gl_file in ]gl_LIBSOURCES_LIST[ ; do if test ! -r ]m4_defn([gl_LIBSOURCES_DIR])[/$gl_file ; then echo "missing file ]m4_defn([gl_LIBSOURCES_DIR])[/$gl_file" >&2 exit 1 fi done])dnl m4_if(m4_sysval, [0], [], [AC_FATAL([expected source file, required through AC_LIBSOURCES, not found])]) ]) m4_popdef([gl_LIBSOURCES_DIR]) m4_popdef([gl_LIBSOURCES_LIST]) m4_popdef([AC_LIBSOURCES]) m4_popdef([AC_REPLACE_FUNCS]) m4_popdef([AC_LIBOBJ]) AC_CONFIG_COMMANDS_PRE([ gl_libobjs= gl_ltlibobjs= if test -n "$gl_LIBOBJS"; then # Remove the extension. sed_drop_objext='s/\.o$//;s/\.obj$//' for i in `for i in $gl_LIBOBJS; do echo "$i"; done | sed -e "$sed_drop_objext" | sort | uniq`; do gl_libobjs="$gl_libobjs $i.$ac_objext" gl_ltlibobjs="$gl_ltlibobjs $i.lo" done fi AC_SUBST([gl_LIBOBJS], [$gl_libobjs]) AC_SUBST([gl_LTLIBOBJS], [$gl_ltlibobjs]) ]) gltests_libdeps= gltests_ltlibdeps= m4_pushdef([AC_LIBOBJ], m4_defn([gltests_LIBOBJ])) m4_pushdef([AC_REPLACE_FUNCS], m4_defn([gltests_REPLACE_FUNCS])) m4_pushdef([AC_LIBSOURCES], m4_defn([gltests_LIBSOURCES])) m4_pushdef([gltests_LIBSOURCES_LIST], []) m4_pushdef([gltests_LIBSOURCES_DIR], []) gl_COMMON gl_source_base='bootstrapped/tests' changequote(,)dnl gltests_WITNESS=IN_`echo "${PACKAGE-$PACKAGE_TARNAME}" | LC_ALL=C tr abcdefghijklmnopqrstuvwxyz ABCDEFGHIJKLMNOPQRSTUVWXYZ | LC_ALL=C sed -e 's/[^A-Z0-9_]/_/g'`_GNULIB_TESTS changequote([, ])dnl AC_SUBST([gltests_WITNESS]) gl_module_indicator_condition=$gltests_WITNESS m4_pushdef([gl_MODULE_INDICATOR_CONDITION], [$gl_module_indicator_condition]) gt_LOCALE_FR gt_LOCALE_FR_UTF8 gt_LOCALE_FR gt_LOCALE_TR_UTF8 gl_FUNC_CLOSE if test $REPLACE_CLOSE = 1; then AC_LIBOBJ([close]) fi gl_UNISTD_MODULE_INDICATOR([close]) gl_CTYPE_H gl_FUNC_DUP2 if test $HAVE_DUP2 = 0 || test $REPLACE_DUP2 = 1; then AC_LIBOBJ([dup2]) gl_PREREQ_DUP2 fi gl_UNISTD_MODULE_INDICATOR([dup2]) gl_ENVIRON gl_UNISTD_MODULE_INDICATOR([environ]) gl_FCNTL_H gl_FUNC_FDOPEN if test $REPLACE_FDOPEN = 1; then AC_LIBOBJ([fdopen]) gl_PREREQ_FDOPEN fi gl_STDIO_MODULE_INDICATOR([fdopen]) AC_C_FLEXIBLE_ARRAY_MEMBER gl_FUNC_FSTAT if test $REPLACE_FSTAT = 1; then AC_LIBOBJ([fstat]) gl_PREREQ_FSTAT fi gl_SYS_STAT_MODULE_INDICATOR([fstat]) gl_FUNC_GETCWD_LGPL if test $REPLACE_GETCWD = 1; then AC_LIBOBJ([getcwd-lgpl]) fi gl_UNISTD_MODULE_INDICATOR([getcwd]) gl_FUNC_GETDTABLESIZE if test $HAVE_GETDTABLESIZE = 0 || test $REPLACE_GETDTABLESIZE = 1; then AC_LIBOBJ([getdtablesize]) gl_PREREQ_GETDTABLESIZE fi gl_UNISTD_MODULE_INDICATOR([getdtablesize]) gl_FUNC_GETPAGESIZE if test $REPLACE_GETPAGESIZE = 1; then AC_LIBOBJ([getpagesize]) fi gl_UNISTD_MODULE_INDICATOR([getpagesize]) gl_FUNC_GETTIMEOFDAY if test $HAVE_GETTIMEOFDAY = 0 || test $REPLACE_GETTIMEOFDAY = 1; then AC_LIBOBJ([gettimeofday]) gl_PREREQ_GETTIMEOFDAY fi gl_SYS_TIME_MODULE_INDICATOR([gettimeofday]) gl_INTTYPES_H gl_INTTYPES_INCOMPLETE AC_REQUIRE([gl_LARGEFILE]) AC_CHECK_FUNCS_ONCE([newlocale]) gl_LOCALENAME AC_CHECK_FUNCS_ONCE([newlocale]) gl_FUNC_LSTAT if test $REPLACE_LSTAT = 1; then AC_LIBOBJ([lstat]) gl_PREREQ_LSTAT fi gl_SYS_STAT_MODULE_INDICATOR([lstat]) gl_MALLOCA gt_LOCALE_FR gt_LOCALE_FR_UTF8 gt_LOCALE_JA gt_LOCALE_ZH_CN gt_LOCALE_FR_UTF8 dnl Check for prerequisites for memory fence checks. gl_FUNC_MMAP_ANON AC_CHECK_HEADERS_ONCE([sys/mman.h]) AC_CHECK_FUNCS_ONCE([mprotect]) gt_LOCALE_FR gt_LOCALE_FR_UTF8 gl_FUNC_OPEN if test $REPLACE_OPEN = 1; then AC_LIBOBJ([open]) gl_PREREQ_OPEN fi gl_FCNTL_MODULE_INDICATOR([open]) gl_PATHMAX gl_FUNC_PUTENV if test $REPLACE_PUTENV = 1; then AC_LIBOBJ([putenv]) gl_PREREQ_PUTENV fi gl_STDLIB_MODULE_INDICATOR([putenv]) dnl Check for prerequisites for memory fence checks. gl_FUNC_MMAP_ANON AC_CHECK_HEADERS_ONCE([sys/mman.h]) AC_CHECK_FUNCS_ONCE([mprotect]) gl_FUNC_SETENV if test $HAVE_SETENV = 0 || test $REPLACE_SETENV = 1; then AC_LIBOBJ([setenv]) fi gl_STDLIB_MODULE_INDICATOR([setenv]) gl_FUNC_SETLOCALE if test $REPLACE_SETLOCALE = 1; then AC_LIBOBJ([setlocale]) gl_PREREQ_SETLOCALE fi gl_LOCALE_MODULE_INDICATOR([setlocale]) gt_LOCALE_FR gt_LOCALE_FR_UTF8 gt_LOCALE_JA gt_LOCALE_ZH_CN AC_CHECK_DECLS_ONCE([alarm]) gl_FUNC_STAT if test $REPLACE_STAT = 1; then AC_LIBOBJ([stat]) gl_PREREQ_STAT fi gl_SYS_STAT_MODULE_INDICATOR([stat]) AC_REQUIRE([gt_TYPE_WCHAR_T]) AC_REQUIRE([gt_TYPE_WINT_T]) dnl Check for prerequisites for memory fence checks. gl_FUNC_MMAP_ANON AC_CHECK_HEADERS_ONCE([sys/mman.h]) AC_CHECK_FUNCS_ONCE([mprotect]) gl_FUNC_SYMLINK if test $HAVE_SYMLINK = 0 || test $REPLACE_SYMLINK = 1; then AC_LIBOBJ([symlink]) fi gl_UNISTD_MODULE_INDICATOR([symlink]) gl_HEADER_SYS_STAT_H AC_PROG_MKDIR_P gl_HEADER_SYS_TIME_H AC_PROG_MKDIR_P gl_THREAD gl_HEADER_TIME_H gl_FUNC_UNSETENV if test $HAVE_UNSETENV = 0 || test $REPLACE_UNSETENV = 1; then AC_LIBOBJ([unsetenv]) gl_PREREQ_UNSETENV fi gl_STDLIB_MODULE_INDICATOR([unsetenv]) gt_LOCALE_FR gt_LOCALE_FR_UTF8 gt_LOCALE_JA gt_LOCALE_ZH_CN gl_FUNC_WCTOB if test $HAVE_WCTOB = 0 || test $REPLACE_WCTOB = 1; then AC_LIBOBJ([wctob]) gl_PREREQ_WCTOB fi gl_WCHAR_MODULE_INDICATOR([wctob]) gl_FUNC_WCTOMB if test $REPLACE_WCTOMB = 1; then AC_LIBOBJ([wctomb]) gl_PREREQ_WCTOMB fi gl_STDLIB_MODULE_INDICATOR([wctomb]) gl_YIELD m4_popdef([gl_MODULE_INDICATOR_CONDITION]) m4_ifval(gltests_LIBSOURCES_LIST, [ m4_syscmd([test ! -d ]m4_defn([gltests_LIBSOURCES_DIR])[ || for gl_file in ]gltests_LIBSOURCES_LIST[ ; do if test ! -r ]m4_defn([gltests_LIBSOURCES_DIR])[/$gl_file ; then echo "missing file ]m4_defn([gltests_LIBSOURCES_DIR])[/$gl_file" >&2 exit 1 fi done])dnl m4_if(m4_sysval, [0], [], [AC_FATAL([expected source file, required through AC_LIBSOURCES, not found])]) ]) m4_popdef([gltests_LIBSOURCES_DIR]) m4_popdef([gltests_LIBSOURCES_LIST]) m4_popdef([AC_LIBSOURCES]) m4_popdef([AC_REPLACE_FUNCS]) m4_popdef([AC_LIBOBJ]) AC_CONFIG_COMMANDS_PRE([ gltests_libobjs= gltests_ltlibobjs= if test -n "$gltests_LIBOBJS"; then # Remove the extension. sed_drop_objext='s/\.o$//;s/\.obj$//' for i in `for i in $gltests_LIBOBJS; do echo "$i"; done | sed -e "$sed_drop_objext" | sort | uniq`; do gltests_libobjs="$gltests_libobjs $i.$ac_objext" gltests_ltlibobjs="$gltests_ltlibobjs $i.lo" done fi AC_SUBST([gltests_LIBOBJS], [$gltests_libobjs]) AC_SUBST([gltests_LTLIBOBJS], [$gltests_ltlibobjs]) ]) LIBTESTS_LIBDEPS="$gltests_libdeps" AC_SUBST([LIBTESTS_LIBDEPS]) ]) # Like AC_LIBOBJ, except that the module name goes # into gl_LIBOBJS instead of into LIBOBJS. AC_DEFUN([gl_LIBOBJ], [ AS_LITERAL_IF([$1], [gl_LIBSOURCES([$1.c])])dnl gl_LIBOBJS="$gl_LIBOBJS $1.$ac_objext" ]) # Like AC_REPLACE_FUNCS, except that the module name goes # into gl_LIBOBJS instead of into LIBOBJS. AC_DEFUN([gl_REPLACE_FUNCS], [ m4_foreach_w([gl_NAME], [$1], [AC_LIBSOURCES(gl_NAME[.c])])dnl AC_CHECK_FUNCS([$1], , [gl_LIBOBJ($ac_func)]) ]) # Like AC_LIBSOURCES, except the directory where the source file is # expected is derived from the gnulib-tool parameterization, # and alloca is special cased (for the alloca-opt module). # We could also entirely rely on EXTRA_lib..._SOURCES. AC_DEFUN([gl_LIBSOURCES], [ m4_foreach([_gl_NAME], [$1], [ m4_if(_gl_NAME, [alloca.c], [], [ m4_define([gl_LIBSOURCES_DIR], [bootstrapped/lib]) m4_append([gl_LIBSOURCES_LIST], _gl_NAME, [ ]) ]) ]) ]) # Like AC_LIBOBJ, except that the module name goes # into gltests_LIBOBJS instead of into LIBOBJS. AC_DEFUN([gltests_LIBOBJ], [ AS_LITERAL_IF([$1], [gltests_LIBSOURCES([$1.c])])dnl gltests_LIBOBJS="$gltests_LIBOBJS $1.$ac_objext" ]) # Like AC_REPLACE_FUNCS, except that the module name goes # into gltests_LIBOBJS instead of into LIBOBJS. AC_DEFUN([gltests_REPLACE_FUNCS], [ m4_foreach_w([gl_NAME], [$1], [AC_LIBSOURCES(gl_NAME[.c])])dnl AC_CHECK_FUNCS([$1], , [gltests_LIBOBJ($ac_func)]) ]) # Like AC_LIBSOURCES, except the directory where the source file is # expected is derived from the gnulib-tool parameterization, # and alloca is special cased (for the alloca-opt module). # We could also entirely rely on EXTRA_lib..._SOURCES. AC_DEFUN([gltests_LIBSOURCES], [ m4_foreach([_gl_NAME], [$1], [ m4_if(_gl_NAME, [alloca.c], [], [ m4_define([gltests_LIBSOURCES_DIR], [bootstrapped/tests]) m4_append([gltests_LIBSOURCES_LIST], _gl_NAME, [ ]) ]) ]) ]) # This macro records the list of files which have been installed by # gnulib-tool and may be removed by future gnulib-tool invocations. AC_DEFUN([gl_FILE_LIST], [ build-aux/config.rpath build-aux/gendocs.sh build-aux/git-version-gen build-aux/snippet/_Noreturn.h build-aux/snippet/arg-nonnull.h build-aux/snippet/c++defs.h build-aux/snippet/warn-on-use.h doc/fdl.texi doc/gendocs_template doc/gendocs_template_min lib/alloca.c lib/alloca.in.h lib/argp-ba.c lib/argp-eexst.c lib/argp-fmtstream.c lib/argp-fmtstream.h lib/argp-fs-xinl.c lib/argp-help.c lib/argp-namefrob.h lib/argp-parse.c lib/argp-pin.c lib/argp-pv.c lib/argp-pvh.c lib/argp-xinl.c lib/argp.h lib/asnprintf.c lib/basename-lgpl.c lib/btowc.c lib/c-ctype.c lib/c-ctype.h lib/config.charset lib/dirname-lgpl.c lib/dirname.h lib/dosname.h lib/errno.in.h lib/error.c lib/error.h lib/float+.h lib/float.c lib/float.in.h lib/getopt.c lib/getopt.in.h lib/getopt1.c lib/getopt_int.h lib/getprogname.c lib/getprogname.h lib/gettext.h lib/glthread/lock.c lib/glthread/lock.h lib/glthread/threadlib.c lib/hard-locale.c lib/hard-locale.h lib/intprops.h lib/itold.c lib/langinfo.in.h lib/limits.in.h lib/localcharset.c lib/localcharset.h lib/locale.in.h lib/localeconv.c lib/malloc.c lib/math.c lib/math.in.h lib/mbrtowc.c lib/mbsinit.c lib/mbtowc-impl.h lib/mbtowc.c lib/memchr.c lib/memchr.valgrind lib/mempcpy.c lib/msvc-inval.c lib/msvc-inval.h lib/msvc-nothrow.c lib/msvc-nothrow.h lib/nl_langinfo.c lib/nproc.c lib/nproc.h lib/printf-args.c lib/printf-args.h lib/printf-parse.c lib/printf-parse.h lib/rawmemchr.c lib/rawmemchr.valgrind lib/ref-add.sin lib/ref-del.sin lib/regcomp.c lib/regex.c lib/regex.h lib/regex_internal.c lib/regex_internal.h lib/regexec.c lib/size_max.h lib/sleep.c lib/stdalign.in.h lib/stdbool.in.h lib/stddef.in.h lib/stdint.in.h lib/stdio.in.h lib/stdlib.in.h lib/strcasecmp.c lib/strchrnul.c lib/strchrnul.valgrind lib/streq.h lib/strerror-override.c lib/strerror-override.h lib/strerror.c lib/string.in.h lib/strings.in.h lib/stripslash.c lib/strncasecmp.c lib/strndup.c lib/strnlen.c lib/sys_types.in.h lib/sysexits.in.h lib/unistd.c lib/unistd.in.h lib/vasnprintf.c lib/vasnprintf.h lib/verify.h lib/vsnprintf.c lib/wchar.in.h lib/wcrtomb.c lib/wctype-h.c lib/wctype.in.h lib/xsize.c lib/xsize.h m4/00gnulib.m4 m4/absolute-header.m4 m4/alloca.m4 m4/argp.m4 m4/btowc.m4 m4/close.m4 m4/codeset.m4 m4/configmake.m4 m4/ctype.m4 m4/dirname.m4 m4/double-slash-root.m4 m4/dup2.m4 m4/eealloc.m4 m4/environ.m4 m4/errno_h.m4 m4/error.m4 m4/exponentd.m4 m4/extensions.m4 m4/extern-inline.m4 m4/fcntl-o.m4 m4/fcntl_h.m4 m4/fdopen.m4 m4/flexmember.m4 m4/float_h.m4 m4/fpieee.m4 m4/fstat.m4 m4/getcwd.m4 m4/getdtablesize.m4 m4/getopt.m4 m4/getpagesize.m4 m4/getprogname.m4 m4/gettimeofday.m4 m4/glibc21.m4 m4/gnulib-common.m4 m4/hard-locale.m4 m4/include_next.m4 m4/intlmacosx.m4 m4/intmax_t.m4 m4/inttypes-pri.m4 m4/inttypes.m4 m4/inttypes_h.m4 m4/langinfo_h.m4 m4/largefile.m4 m4/lcmessage.m4 m4/lib-ld.m4 m4/lib-link.m4 m4/lib-prefix.m4 m4/limits-h.m4 m4/localcharset.m4 m4/locale-fr.m4 m4/locale-ja.m4 m4/locale-tr.m4 m4/locale-zh.m4 m4/locale_h.m4 m4/localeconv.m4 m4/localename.m4 m4/lock.m4 m4/longlong.m4 m4/lstat.m4 m4/malloc.m4 m4/malloca.m4 m4/math_h.m4 m4/mbrtowc.m4 m4/mbsinit.m4 m4/mbstate_t.m4 m4/mbtowc.m4 m4/memchr.m4 m4/mempcpy.m4 m4/mmap-anon.m4 m4/mode_t.m4 m4/msvc-inval.m4 m4/msvc-nothrow.m4 m4/multiarch.m4 m4/nl_langinfo.m4 m4/nocrash.m4 m4/nproc.m4 m4/off_t.m4 m4/open.m4 m4/pathmax.m4 m4/printf.m4 m4/putenv.m4 m4/rawmemchr.m4 m4/regex.m4 m4/setenv.m4 m4/setlocale.m4 m4/size_max.m4 m4/sleep.m4 m4/ssize_t.m4 m4/stat.m4 m4/stdalign.m4 m4/stdbool.m4 m4/stddef_h.m4 m4/stdint.m4 m4/stdint_h.m4 m4/stdio_h.m4 m4/stdlib_h.m4 m4/strcase.m4 m4/strchrnul.m4 m4/strerror.m4 m4/string_h.m4 m4/strings_h.m4 m4/strndup.m4 m4/strnlen.m4 m4/symlink.m4 m4/sys_socket_h.m4 m4/sys_stat_h.m4 m4/sys_time_h.m4 m4/sys_types_h.m4 m4/sysexits.m4 m4/thread.m4 m4/threadlib.m4 m4/time_h.m4 m4/unistd_h.m4 m4/vasnprintf.m4 m4/vsnprintf.m4 m4/warn-on-use.m4 m4/wchar_h.m4 m4/wchar_t.m4 m4/wcrtomb.m4 m4/wctob.m4 m4/wctomb.m4 m4/wctype_h.m4 m4/wint_t.m4 m4/xsize.m4 m4/yield.m4 tests/init.sh tests/macros.h tests/signature.h tests/test-alloca-opt.c tests/test-argp-2.sh tests/test-argp.c tests/test-binary-io.c tests/test-binary-io.sh tests/test-btowc.c tests/test-btowc1.sh tests/test-btowc2.sh tests/test-c-ctype.c tests/test-c-strcase.sh tests/test-c-strcasecmp.c tests/test-c-strncasecmp.c tests/test-close.c tests/test-ctype.c tests/test-dup2.c tests/test-environ.c tests/test-errno.c tests/test-fcntl-h.c tests/test-fdopen.c tests/test-fgetc.c tests/test-float.c tests/test-fputc.c tests/test-fread.c tests/test-fstat.c tests/test-fwrite.c tests/test-getcwd-lgpl.c tests/test-getdtablesize.c tests/test-getopt.c tests/test-getopt.h tests/test-getopt_long.h tests/test-getprogname.c tests/test-gettimeofday.c tests/test-ignore-value.c tests/test-init.sh tests/test-intprops.c tests/test-inttypes.c tests/test-langinfo.c tests/test-limits-h.c tests/test-locale.c tests/test-localeconv.c tests/test-localename.c tests/test-lock.c tests/test-lstat.c tests/test-lstat.h tests/test-malloc-gnu.c tests/test-malloca.c tests/test-math.c tests/test-mbrtowc-w32-1.sh tests/test-mbrtowc-w32-2.sh tests/test-mbrtowc-w32-3.sh tests/test-mbrtowc-w32-4.sh tests/test-mbrtowc-w32-5.sh tests/test-mbrtowc-w32.c tests/test-mbrtowc.c tests/test-mbrtowc1.sh tests/test-mbrtowc2.sh tests/test-mbrtowc3.sh tests/test-mbrtowc4.sh tests/test-mbrtowc5.sh tests/test-mbsinit.c tests/test-mbsinit.sh tests/test-memchr.c tests/test-nl_langinfo.c tests/test-nl_langinfo.sh tests/test-open.c tests/test-open.h tests/test-pathmax.c tests/test-rawmemchr.c tests/test-regex.c tests/test-setenv.c tests/test-setlocale1.c tests/test-setlocale1.sh tests/test-setlocale2.c tests/test-setlocale2.sh tests/test-sleep.c tests/test-stat.c tests/test-stat.h tests/test-stdalign.c tests/test-stdbool.c tests/test-stddef.c tests/test-stdint.c tests/test-stdio.c tests/test-stdlib.c tests/test-strchrnul.c tests/test-strerror.c tests/test-string.c tests/test-strings.c tests/test-strnlen.c tests/test-symlink.c tests/test-symlink.h tests/test-sys_stat.c tests/test-sys_time.c tests/test-sys_types.c tests/test-sys_wait.h tests/test-sysexits.c tests/test-thread_create.c tests/test-thread_self.c tests/test-time.c tests/test-unistd.c tests/test-unsetenv.c tests/test-vasnprintf.c tests/test-verify.c tests/test-verify.sh tests/test-vsnprintf.c tests/test-wchar.c tests/test-wcrtomb-w32-1.sh tests/test-wcrtomb-w32-2.sh tests/test-wcrtomb-w32-3.sh tests/test-wcrtomb-w32-4.sh tests/test-wcrtomb-w32-5.sh tests/test-wcrtomb-w32.c tests/test-wcrtomb.c tests/test-wcrtomb.sh tests/test-wctype-h.c tests/zerosize-ptr.h tests=lib/binary-io.c tests=lib/binary-io.h tests=lib/c-strcase.h tests=lib/c-strcasecmp.c tests=lib/c-strncasecmp.c tests=lib/close.c tests=lib/ctype.in.h tests=lib/dup2.c tests=lib/fcntl.in.h tests=lib/fd-hook.c tests=lib/fd-hook.h tests=lib/fdopen.c tests=lib/flexmember.h tests=lib/fpucw.h tests=lib/fstat.c tests=lib/getcwd-lgpl.c tests=lib/getdtablesize.c tests=lib/getpagesize.c tests=lib/gettimeofday.c tests=lib/glthread/thread.c tests=lib/glthread/thread.h tests=lib/glthread/yield.h tests=lib/ignore-value.h tests=lib/inttypes.in.h tests=lib/localename.c tests=lib/localename.h tests=lib/lstat.c tests=lib/malloca.c tests=lib/malloca.h tests=lib/malloca.valgrind tests=lib/open.c tests=lib/pathmax.h tests=lib/putenv.c tests=lib/same-inode.h tests=lib/setenv.c tests=lib/setlocale.c tests=lib/stat.c tests=lib/symlink.c tests=lib/sys_stat.in.h tests=lib/sys_time.in.h tests=lib/time.in.h tests=lib/unsetenv.c tests=lib/wctob.c tests=lib/wctomb-impl.h tests=lib/wctomb.c ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/gnulib-common.m40000644000175000017500000004261213004436754017166 00000000000000# gnulib-common.m4 serial 36 dnl Copyright (C) 2007-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # gl_COMMON # is expanded unconditionally through gnulib-tool magic. AC_DEFUN([gl_COMMON], [ dnl Use AC_REQUIRE here, so that the code is expanded once only. AC_REQUIRE([gl_00GNULIB]) AC_REQUIRE([gl_COMMON_BODY]) ]) AC_DEFUN([gl_COMMON_BODY], [ AH_VERBATIM([_Noreturn], [/* The _Noreturn keyword of C11. */ #if ! (defined _Noreturn \ || (defined __STDC_VERSION__ && 201112 <= __STDC_VERSION__)) # if (3 <= __GNUC__ || (__GNUC__ == 2 && 8 <= __GNUC_MINOR__) \ || 0x5110 <= __SUNPRO_C) # define _Noreturn __attribute__ ((__noreturn__)) # elif defined _MSC_VER && 1200 <= _MSC_VER # define _Noreturn __declspec (noreturn) # else # define _Noreturn # endif #endif ]) AH_VERBATIM([isoc99_inline], [/* Work around a bug in Apple GCC 4.0.1 build 5465: In C99 mode, it supports the ISO C 99 semantics of 'extern inline' (unlike the GNU C semantics of earlier versions), but does not display it by setting __GNUC_STDC_INLINE__. __APPLE__ && __MACH__ test for Mac OS X. __APPLE_CC__ tests for the Apple compiler and its version. __STDC_VERSION__ tests for the C99 mode. */ #if defined __APPLE__ && defined __MACH__ && __APPLE_CC__ >= 5465 && !defined __cplusplus && __STDC_VERSION__ >= 199901L && !defined __GNUC_STDC_INLINE__ # define __GNUC_STDC_INLINE__ 1 #endif]) AH_VERBATIM([unused_parameter], [/* Define as a marker that can be attached to declarations that might not be used. This helps to reduce warnings, such as from GCC -Wunused-parameter. */ #if __GNUC__ >= 3 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 7) # define _GL_UNUSED __attribute__ ((__unused__)) #else # define _GL_UNUSED #endif /* The name _UNUSED_PARAMETER_ is an earlier spelling, although the name is a misnomer outside of parameter lists. */ #define _UNUSED_PARAMETER_ _GL_UNUSED /* gcc supports the "unused" attribute on possibly unused labels, and g++ has since version 4.5. Note to support C++ as well as C, _GL_UNUSED_LABEL should be used with a trailing ; */ #if !defined __cplusplus || __GNUC__ > 4 \ || (__GNUC__ == 4 && __GNUC_MINOR__ >= 5) # define _GL_UNUSED_LABEL _GL_UNUSED #else # define _GL_UNUSED_LABEL #endif /* The __pure__ attribute was added in gcc 2.96. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 96) # define _GL_ATTRIBUTE_PURE __attribute__ ((__pure__)) #else # define _GL_ATTRIBUTE_PURE /* empty */ #endif /* The __const__ attribute was added in gcc 2.95. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 95) # define _GL_ATTRIBUTE_CONST __attribute__ ((__const__)) #else # define _GL_ATTRIBUTE_CONST /* empty */ #endif ]) dnl Preparation for running test programs: dnl Tell glibc to write diagnostics from -D_FORTIFY_SOURCE=2 to stderr, not dnl to /dev/tty, so they can be redirected to log files. Such diagnostics dnl arise e.g., in the macros gl_PRINTF_DIRECTIVE_N, gl_SNPRINTF_DIRECTIVE_N. LIBC_FATAL_STDERR_=1 export LIBC_FATAL_STDERR_ ]) # gl_MODULE_INDICATOR_CONDITION # expands to a C preprocessor expression that evaluates to 1 or 0, depending # whether a gnulib module that has been requested shall be considered present # or not. m4_define([gl_MODULE_INDICATOR_CONDITION], [1]) # gl_MODULE_INDICATOR_SET_VARIABLE([modulename]) # sets the shell variable that indicates the presence of the given module to # a C preprocessor expression that will evaluate to 1. AC_DEFUN([gl_MODULE_INDICATOR_SET_VARIABLE], [ gl_MODULE_INDICATOR_SET_VARIABLE_AUX( [GNULIB_[]m4_translit([[$1]], [abcdefghijklmnopqrstuvwxyz./-], [ABCDEFGHIJKLMNOPQRSTUVWXYZ___])], [gl_MODULE_INDICATOR_CONDITION]) ]) # gl_MODULE_INDICATOR_SET_VARIABLE_AUX([variable]) # modifies the shell variable to include the gl_MODULE_INDICATOR_CONDITION. # The shell variable's value is a C preprocessor expression that evaluates # to 0 or 1. AC_DEFUN([gl_MODULE_INDICATOR_SET_VARIABLE_AUX], [ m4_if(m4_defn([gl_MODULE_INDICATOR_CONDITION]), [1], [ dnl Simplify the expression VALUE || 1 to 1. $1=1 ], [gl_MODULE_INDICATOR_SET_VARIABLE_AUX_OR([$1], [gl_MODULE_INDICATOR_CONDITION])]) ]) # gl_MODULE_INDICATOR_SET_VARIABLE_AUX_OR([variable], [condition]) # modifies the shell variable to include the given condition. The shell # variable's value is a C preprocessor expression that evaluates to 0 or 1. AC_DEFUN([gl_MODULE_INDICATOR_SET_VARIABLE_AUX_OR], [ dnl Simplify the expression 1 || CONDITION to 1. if test "$[]$1" != 1; then dnl Simplify the expression 0 || CONDITION to CONDITION. if test "$[]$1" = 0; then $1=$2 else $1="($[]$1 || $2)" fi fi ]) # gl_MODULE_INDICATOR([modulename]) # defines a C macro indicating the presence of the given module # in a location where it can be used. # | Value | Value | # | in lib/ | in tests/ | # --------------------------------------------+---------+-----------+ # Module present among main modules: | 1 | 1 | # --------------------------------------------+---------+-----------+ # Module present among tests-related modules: | 0 | 1 | # --------------------------------------------+---------+-----------+ # Module not present at all: | 0 | 0 | # --------------------------------------------+---------+-----------+ AC_DEFUN([gl_MODULE_INDICATOR], [ AC_DEFINE_UNQUOTED([GNULIB_]m4_translit([[$1]], [abcdefghijklmnopqrstuvwxyz./-], [ABCDEFGHIJKLMNOPQRSTUVWXYZ___]), [gl_MODULE_INDICATOR_CONDITION], [Define to a C preprocessor expression that evaluates to 1 or 0, depending whether the gnulib module $1 shall be considered present.]) ]) # gl_MODULE_INDICATOR_FOR_TESTS([modulename]) # defines a C macro indicating the presence of the given module # in lib or tests. This is useful to determine whether the module # should be tested. # | Value | Value | # | in lib/ | in tests/ | # --------------------------------------------+---------+-----------+ # Module present among main modules: | 1 | 1 | # --------------------------------------------+---------+-----------+ # Module present among tests-related modules: | 1 | 1 | # --------------------------------------------+---------+-----------+ # Module not present at all: | 0 | 0 | # --------------------------------------------+---------+-----------+ AC_DEFUN([gl_MODULE_INDICATOR_FOR_TESTS], [ AC_DEFINE([GNULIB_TEST_]m4_translit([[$1]], [abcdefghijklmnopqrstuvwxyz./-], [ABCDEFGHIJKLMNOPQRSTUVWXYZ___]), [1], [Define to 1 when the gnulib module $1 should be tested.]) ]) # gl_ASSERT_NO_GNULIB_POSIXCHECK # asserts that there will never be a need to #define GNULIB_POSIXCHECK. # and thereby enables an optimization of configure and config.h. # Used by Emacs. AC_DEFUN([gl_ASSERT_NO_GNULIB_POSIXCHECK], [ dnl Override gl_WARN_ON_USE_PREPARE. dnl But hide this definition from 'aclocal'. AC_DEFUN([gl_W][ARN_ON_USE_PREPARE], []) ]) # gl_ASSERT_NO_GNULIB_TESTS # asserts that there will be no gnulib tests in the scope of the configure.ac # and thereby enables an optimization of config.h. # Used by Emacs. AC_DEFUN([gl_ASSERT_NO_GNULIB_TESTS], [ dnl Override gl_MODULE_INDICATOR_FOR_TESTS. AC_DEFUN([gl_MODULE_INDICATOR_FOR_TESTS], []) ]) # Test whether exists. # Set HAVE_FEATURES_H. AC_DEFUN([gl_FEATURES_H], [ AC_CHECK_HEADERS_ONCE([features.h]) if test $ac_cv_header_features_h = yes; then HAVE_FEATURES_H=1 else HAVE_FEATURES_H=0 fi AC_SUBST([HAVE_FEATURES_H]) ]) # m4_foreach_w # is a backport of autoconf-2.59c's m4_foreach_w. # Remove this macro when we can assume autoconf >= 2.60. m4_ifndef([m4_foreach_w], [m4_define([m4_foreach_w], [m4_foreach([$1], m4_split(m4_normalize([$2]), [ ]), [$3])])]) # AS_VAR_IF(VAR, VALUE, [IF-MATCH], [IF-NOT-MATCH]) # ---------------------------------------------------- # Backport of autoconf-2.63b's macro. # Remove this macro when we can assume autoconf >= 2.64. m4_ifndef([AS_VAR_IF], [m4_define([AS_VAR_IF], [AS_IF([test x"AS_VAR_GET([$1])" = x""$2], [$3], [$4])])]) # gl_PROG_CC_C99 # Modifies the value of the shell variable CC in an attempt to make $CC # understand ISO C99 source code. # This is like AC_PROG_CC_C99, except that # - AC_PROG_CC_C99 did not exist in Autoconf versions < 2.60, # - AC_PROG_CC_C99 does not mix well with AC_PROG_CC_STDC # , # but many more packages use AC_PROG_CC_STDC than AC_PROG_CC_C99 # . # Remaining problems: # - When AC_PROG_CC_STDC is invoked twice, it adds the C99 enabling options # to CC twice # . # - AC_PROG_CC_STDC is likely to change now that C11 is an ISO standard. 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AC_DEFUN([gl_BIGENDIAN], [ AC_C_BIGENDIAN ]) # gl_CACHE_VAL_SILENT(cache-id, command-to-set-it) # is like AC_CACHE_VAL(cache-id, command-to-set-it), except that it does not # output a spurious "(cached)" mark in the midst of other configure output. # This macro should be used instead of AC_CACHE_VAL when it is not surrounded # by an AC_MSG_CHECKING/AC_MSG_RESULT pair. AC_DEFUN([gl_CACHE_VAL_SILENT], [ saved_as_echo_n="$as_echo_n" as_echo_n=':' AC_CACHE_VAL([$1], [$2]) as_echo_n="$saved_as_echo_n" ]) # AS_VAR_COPY was added in autoconf 2.63b m4_define_default([AS_VAR_COPY], [AS_LITERAL_IF([$1[]$2], [$1=$$2], [eval $1=\$$2])]) # AC_PROG_SED was added in autoconf 2.59b m4_ifndef([AC_PROG_SED], [AC_DEFUN([AC_PROG_SED], [AC_CACHE_CHECK([for a sed that does not truncate output], ac_cv_path_SED, [dnl ac_script should not contain more than 99 commands (for HP-UX sed), dnl but more than about 7000 bytes, to catch a limit in Solaris 8 /usr/ucb/sed. ac_script=s/aaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaa/bbbbbbbbbbbbbbbbbbbbbbbbbbbbbbbbb/ for ac_i in 1 2 3 4 5 6 7; do ac_script="$ac_script$as_nl$ac_script" done echo "$ac_script" 2>/dev/null | sed 99q >conftest.sed AS_UNSET([ac_script]) if test -z "$SED"; then ac_path_SED_found=false _AS_PATH_WALK([], [ for ac_prog in sed gsed; do for ac_exec_ext in '' $ac_executable_extensions; do ac_path_SED="$as_dir/$ac_prog$ac_exec_ext" AS_EXECUTABLE_P(["$ac_path_SED"]) || continue case `"$ac_path_SED" --version 2>&1` in *GNU*) ac_cv_path_SED=$ac_path_SED ac_path_SED_found=:;; *) ac_count=0 _AS_ECHO_N([0123456789]) >conftest.in while : do cat conftest.in conftest.in >conftest.tmp mv conftest.tmp conftest.in cp conftest.in conftest.nl echo >> conftest.nl "$ac_path_SED" -f conftest.sed conftest.out 2>/dev/null || break diff conftest.out conftest.nl >/dev/null 2>&1 || break ac_count=`expr $ac_count + 1` if test $ac_count -gt ${ac_path_SED_max-0}; then # Best so far, but keep looking for better ac_cv_path_SED=$ac_path_SED ac_path_SED_max=$ac_count fi test $ac_count -gt 10 && break done rm -f conftest.in conftest.tmp conftest.nl conftest.out;; esac $ac_path_SED_found && break 3 done done]) if test -z "$ac_cv_path_SED"; then AC_ERROR([no acceptable sed could be found in \$PATH]) fi else ac_cv_path_SED=$SED fi SED="$ac_cv_path_SED" AC_SUBST([SED])dnl rm -f conftest.sed ])])]) gnuastro-0.2.33-8a3b/bootstrapped/m4/glibc21.m40000644000175000017500000000161313004436754015637 00000000000000# glibc21.m4 serial 5 dnl Copyright (C) 2000-2002, 2004, 2008, 2010-2016 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # Test for the GNU C Library, version 2.1 or newer, or uClibc. # From Bruno Haible. AC_DEFUN([gl_GLIBC21], [ AC_CACHE_CHECK([whether we are using the GNU C Library >= 2.1 or uClibc], [ac_cv_gnu_library_2_1], [AC_EGREP_CPP([Lucky], [ #include #ifdef __GNU_LIBRARY__ #if (__GLIBC__ == 2 && __GLIBC_MINOR__ >= 1) || (__GLIBC__ > 2) Lucky GNU user #endif #endif #ifdef __UCLIBC__ Lucky user #endif ], [ac_cv_gnu_library_2_1=yes], [ac_cv_gnu_library_2_1=no]) ] ) AC_SUBST([GLIBC21]) GLIBC21="$ac_cv_gnu_library_2_1" ] ) gnuastro-0.2.33-8a3b/bootstrapped/m4/gettimeofday.m40000644000175000017500000001143513004436754017100 00000000000000# serial 21 # Copyright (C) 2001-2003, 2005, 2007, 2009-2016 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. dnl From Jim Meyering. AC_DEFUN([gl_FUNC_GETTIMEOFDAY], [ AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([gl_HEADER_SYS_TIME_H]) AC_REQUIRE([gl_HEADER_SYS_TIME_H_DEFAULTS]) AC_CHECK_FUNCS_ONCE([gettimeofday]) gl_gettimeofday_timezone=void if test $ac_cv_func_gettimeofday != yes; then HAVE_GETTIMEOFDAY=0 else gl_FUNC_GETTIMEOFDAY_CLOBBER AC_CACHE_CHECK([for gettimeofday with POSIX signature], [gl_cv_func_gettimeofday_posix_signature], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include struct timeval c; int gettimeofday (struct timeval *restrict, void *restrict); ]], [[/* glibc uses struct timezone * rather than the POSIX void * if _GNU_SOURCE is defined. However, since the only portable use of gettimeofday uses NULL as the second parameter, and since the glibc definition is actually more typesafe, it is not worth wrapping this to get a compliant signature. */ int (*f) (struct timeval *restrict, void *restrict) = gettimeofday; int x = f (&c, 0); return !(x | c.tv_sec | c.tv_usec); ]])], [gl_cv_func_gettimeofday_posix_signature=yes], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include int gettimeofday (struct timeval *restrict, struct timezone *restrict); ]])], [gl_cv_func_gettimeofday_posix_signature=almost], [gl_cv_func_gettimeofday_posix_signature=no])])]) if test $gl_cv_func_gettimeofday_posix_signature = almost; then gl_gettimeofday_timezone='struct timezone' elif test $gl_cv_func_gettimeofday_posix_signature != yes; then REPLACE_GETTIMEOFDAY=1 fi dnl If we override 'struct timeval', we also have to override gettimeofday. if test $REPLACE_STRUCT_TIMEVAL = 1; then REPLACE_GETTIMEOFDAY=1 fi m4_ifdef([gl_FUNC_TZSET_CLOBBER], [ gl_FUNC_TZSET_CLOBBER case "$gl_cv_func_tzset_clobber" in *yes) REPLACE_GETTIMEOFDAY=1 gl_GETTIMEOFDAY_REPLACE_LOCALTIME AC_DEFINE([tzset], [rpl_tzset], [Define to rpl_tzset if the wrapper function should be used.]) AC_DEFINE([TZSET_CLOBBERS_LOCALTIME], [1], [Define if tzset clobbers localtime's static buffer.]) ;; esac ]) fi AC_DEFINE_UNQUOTED([GETTIMEOFDAY_TIMEZONE], [$gl_gettimeofday_timezone], [Define this to 'void' or 'struct timezone' to match the system's declaration of the second argument to gettimeofday.]) ]) dnl See if gettimeofday clobbers the static buffer that localtime uses dnl for its return value. The gettimeofday function from Mac OS X 10.0.4 dnl (i.e., Darwin 1.3.7) has this problem. dnl dnl If it does, then arrange to use gettimeofday and localtime only via dnl the wrapper functions that work around the problem. AC_DEFUN([gl_FUNC_GETTIMEOFDAY_CLOBBER], [ AC_REQUIRE([gl_HEADER_SYS_TIME_H]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether gettimeofday clobbers localtime buffer], [gl_cv_func_gettimeofday_clobber], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include #include #include ]], [[ time_t t = 0; struct tm *lt; struct tm saved_lt; struct timeval tv; lt = localtime (&t); saved_lt = *lt; gettimeofday (&tv, NULL); return memcmp (lt, &saved_lt, sizeof (struct tm)) != 0; ]])], [gl_cv_func_gettimeofday_clobber=no], [gl_cv_func_gettimeofday_clobber=yes], [# When cross-compiling: case "$host_os" in # Guess all is fine on glibc systems. *-gnu*) gl_cv_func_gettimeofday_clobber="guessing no" ;; # If we don't know, assume the worst. *) gl_cv_func_gettimeofday_clobber="guessing yes" ;; esac ])]) case "$gl_cv_func_gettimeofday_clobber" in *yes) REPLACE_GETTIMEOFDAY=1 gl_GETTIMEOFDAY_REPLACE_LOCALTIME AC_DEFINE([GETTIMEOFDAY_CLOBBERS_LOCALTIME], [1], [Define if gettimeofday clobbers the localtime buffer.]) ;; esac ]) AC_DEFUN([gl_GETTIMEOFDAY_REPLACE_LOCALTIME], [ REPLACE_GMTIME=1 REPLACE_LOCALTIME=1 ]) # Prerequisites of lib/gettimeofday.c. AC_DEFUN([gl_PREREQ_GETTIMEOFDAY], [ AC_CHECK_HEADERS([sys/timeb.h]) AC_CHECK_FUNCS([_ftime]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/getprogname.m40000644000175000017500000000262613004436754016731 00000000000000# getprogname.m4 - check for getprogname or replacements for it # Copyright (C) 2016 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # serial 4 AC_DEFUN([gl_FUNC_GETPROGNAME], [ AC_CHECK_FUNCS_ONCE([getprogname getexecname]) AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) ac_found=0 AC_CHECK_DECLS([program_invocation_name], [ac_found=1], [], [#include ]) AC_CHECK_DECLS([program_invocation_short_name], [ac_found=1], [], [#include ]) AC_CHECK_DECLS([__argv], [ac_found=1], [], [#include ]) # Incur the cost of this test only if none of the above worked. if test $ac_found = 0; then # On OpenBSD 5.1, using the global __progname variable appears to be # the only way to implement getprogname. AC_CACHE_CHECK([whether __progname is defined in default libraries], [gl_cv_var___progname], [ gl_cv_var___progname= AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[extern char *__progname;]], [[return *__progname;]] )], [gl_cv_var___progname=yes] ) ] ) if test "$gl_cv_var___progname" = yes; then AC_DEFINE([HAVE_VAR___PROGNAME], 1, [Define if you have a global __progname variable]) fi fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/getpagesize.m40000644000175000017500000000172213004436754016724 00000000000000# getpagesize.m4 serial 9 dnl Copyright (C) 2002, 2004-2005, 2007, 2009-2016 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_GETPAGESIZE], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) AC_CHECK_FUNCS([getpagesize]) if test $ac_cv_func_getpagesize = no; then HAVE_GETPAGESIZE=0 AC_CHECK_HEADERS([OS.h]) if test $ac_cv_header_OS_h = yes; then HAVE_OS_H=1 fi AC_CHECK_HEADERS([sys/param.h]) if test $ac_cv_header_sys_param_h = yes; then HAVE_SYS_PARAM_H=1 fi fi case "$host_os" in mingw*) REPLACE_GETPAGESIZE=1 ;; esac dnl Also check whether it's declared. dnl mingw has getpagesize() in libgcc.a but doesn't declare it. AC_CHECK_DECL([getpagesize], , [HAVE_DECL_GETPAGESIZE=0]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/getopt.m40000644000175000017500000003013413004436754015716 00000000000000# getopt.m4 serial 44 dnl Copyright (C) 2002-2006, 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # Request a POSIX compliant getopt function. AC_DEFUN([gl_FUNC_GETOPT_POSIX], [ m4_divert_text([DEFAULTS], [gl_getopt_required=POSIX]) AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([gl_GETOPT_CHECK_HEADERS]) dnl Other modules can request the gnulib implementation of the getopt dnl functions unconditionally, by defining gl_REPLACE_GETOPT_ALWAYS. dnl argp.m4 does this. m4_ifdef([gl_REPLACE_GETOPT_ALWAYS], [ REPLACE_GETOPT=1 ], [ REPLACE_GETOPT=0 if test -n "$gl_replace_getopt"; then REPLACE_GETOPT=1 fi ]) if test $REPLACE_GETOPT = 1; then dnl Arrange for getopt.h to be created. gl_GETOPT_SUBSTITUTE_HEADER fi ]) # Request a POSIX compliant getopt function with GNU extensions (such as # options with optional arguments) and the functions getopt_long, # getopt_long_only. AC_DEFUN([gl_FUNC_GETOPT_GNU], [ m4_divert_text([INIT_PREPARE], [gl_getopt_required=GNU]) AC_REQUIRE([gl_FUNC_GETOPT_POSIX]) ]) # Determine whether to replace the entire getopt facility. AC_DEFUN([gl_GETOPT_CHECK_HEADERS], [ AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([AC_PROG_AWK]) dnl for awk that supports ENVIRON dnl Persuade Solaris to declare optarg, optind, opterr, optopt. AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) gl_CHECK_NEXT_HEADERS([getopt.h]) if test $ac_cv_header_getopt_h = yes; then HAVE_GETOPT_H=1 else HAVE_GETOPT_H=0 fi AC_SUBST([HAVE_GETOPT_H]) gl_replace_getopt= dnl Test whether is available. if test -z "$gl_replace_getopt" && test $gl_getopt_required = GNU; then AC_CHECK_HEADERS([getopt.h], [], [gl_replace_getopt=yes]) fi dnl Test whether the function getopt_long is available. if test -z "$gl_replace_getopt" && test $gl_getopt_required = GNU; then AC_CHECK_FUNCS([getopt_long_only], [], [gl_replace_getopt=yes]) fi dnl POSIX 2008 does not specify leading '+' behavior, but see dnl http://austingroupbugs.net/view.php?id=191 for a recommendation on dnl the next version of POSIX. For now, we only guarantee leading '+' dnl behavior with getopt-gnu. if test -z "$gl_replace_getopt"; then AC_CACHE_CHECK([whether getopt is POSIX compatible], [gl_cv_func_getopt_posix], [ dnl Merging these three different test programs into a single one dnl would require a reset mechanism. On BSD systems, it can be done dnl through 'optreset'; on some others (glibc), it can be done by dnl setting 'optind' to 0; on others again (HP-UX, IRIX, OSF/1, dnl Solaris 9, musl libc), there is no such mechanism. if test $cross_compiling = no; then dnl Sanity check. Succeeds everywhere (except on MSVC, dnl which lacks and getopt() entirely). AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include int main () { static char program[] = "program"; static char a[] = "-a"; static char foo[] = "foo"; static char bar[] = "bar"; char *argv[] = { program, a, foo, bar, NULL }; int c; c = getopt (4, argv, "ab"); if (!(c == 'a')) return 1; c = getopt (4, argv, "ab"); if (!(c == -1)) return 2; if (!(optind == 2)) return 3; return 0; } ]])], [gl_cv_func_getopt_posix=maybe], [gl_cv_func_getopt_posix=no]) if test $gl_cv_func_getopt_posix = maybe; then dnl Sanity check with '+'. Succeeds everywhere (except on MSVC, dnl which lacks and getopt() entirely). AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include int main () { static char program[] = "program"; static char donald[] = "donald"; static char p[] = "-p"; static char billy[] = "billy"; static char duck[] = "duck"; static char a[] = "-a"; static char bar[] = "bar"; char *argv[] = { program, donald, p, billy, duck, a, bar, NULL }; int c; c = getopt (7, argv, "+abp:q:"); if (!(c == -1)) return 4; if (!(strcmp (argv[0], "program") == 0)) return 5; if (!(strcmp (argv[1], "donald") == 0)) return 6; if (!(strcmp (argv[2], "-p") == 0)) return 7; if (!(strcmp (argv[3], "billy") == 0)) return 8; if (!(strcmp (argv[4], "duck") == 0)) return 9; if (!(strcmp (argv[5], "-a") == 0)) return 10; if (!(strcmp (argv[6], "bar") == 0)) return 11; if (!(optind == 1)) return 12; return 0; } ]])], [gl_cv_func_getopt_posix=maybe], [gl_cv_func_getopt_posix=no]) fi if test $gl_cv_func_getopt_posix = maybe; then dnl Detect Mac OS X 10.5, AIX 7.1, mingw bug. AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include int main () { static char program[] = "program"; static char ab[] = "-ab"; char *argv[3] = { program, ab, NULL }; if (getopt (2, argv, "ab:") != 'a') return 13; if (getopt (2, argv, "ab:") != '?') return 14; if (optopt != 'b') return 15; if (optind != 2) return 16; return 0; } ]])], [gl_cv_func_getopt_posix=yes], [gl_cv_func_getopt_posix=no]) fi else case "$host_os" in darwin* | aix* | mingw*) gl_cv_func_getopt_posix="guessing no";; *) gl_cv_func_getopt_posix="guessing yes";; esac fi ]) case "$gl_cv_func_getopt_posix" in *no) gl_replace_getopt=yes ;; esac fi if test -z "$gl_replace_getopt" && test $gl_getopt_required = GNU; then AC_CACHE_CHECK([for working GNU getopt function], [gl_cv_func_getopt_gnu], [# Even with POSIXLY_CORRECT, the GNU extension of leading '-' in the # optstring is necessary for programs like m4 that have POSIX-mandated # semantics for supporting options interspersed with files. # Also, since getopt_long is a GNU extension, we require optind=0. # Bash ties 'set -o posix' to a non-exported POSIXLY_CORRECT; # so take care to revert to the correct (non-)export state. dnl GNU Coding Standards currently allow awk but not env; besides, env dnl is ambiguous with environment values that contain newlines. gl_awk_probe='BEGIN { if ("POSIXLY_CORRECT" in ENVIRON) print "x" }' case ${POSIXLY_CORRECT+x}`$AWK "$gl_awk_probe" #include #include ]GL_NOCRASH[ ]], [[ int result = 0; nocrash_init(); /* This code succeeds on glibc 2.8, OpenBSD 4.0, Cygwin, mingw, and fails on Mac OS X 10.5, AIX 5.2, HP-UX 11, IRIX 6.5, OSF/1 5.1, Solaris 10. */ { static char conftest[] = "conftest"; static char plus[] = "-+"; char *argv[3] = { conftest, plus, NULL }; opterr = 0; if (getopt (2, argv, "+a") != '?') result |= 1; } /* This code succeeds on glibc 2.8, mingw, and fails on Mac OS X 10.5, OpenBSD 4.0, AIX 5.2, HP-UX 11, IRIX 6.5, OSF/1 5.1, Solaris 10, Cygwin 1.5.x. */ { static char program[] = "program"; static char p[] = "-p"; static char foo[] = "foo"; static char bar[] = "bar"; char *argv[] = { program, p, foo, bar, NULL }; optind = 1; if (getopt (4, argv, "p::") != 'p') result |= 2; else if (optarg != NULL) result |= 4; else if (getopt (4, argv, "p::") != -1) result |= 6; else if (optind != 2) result |= 8; } /* This code succeeds on glibc 2.8 and fails on Cygwin 1.7.0. */ { static char program[] = "program"; static char foo[] = "foo"; static char p[] = "-p"; char *argv[] = { program, foo, p, NULL }; optind = 0; if (getopt (3, argv, "-p") != 1) result |= 16; else if (getopt (3, argv, "-p") != 'p') result |= 16; } /* This code fails on glibc 2.11. */ { static char program[] = "program"; static char b[] = "-b"; static char a[] = "-a"; char *argv[] = { program, b, a, NULL }; optind = opterr = 0; if (getopt (3, argv, "+:a:b") != 'b') result |= 32; else if (getopt (3, argv, "+:a:b") != ':') result |= 32; } /* This code dumps core on glibc 2.14. */ { static char program[] = "program"; static char w[] = "-W"; static char dummy[] = "dummy"; char *argv[] = { program, w, dummy, NULL }; optind = opterr = 1; if (getopt (3, argv, "W;") != 'W') result |= 64; } return result; ]])], [gl_cv_func_getopt_gnu=yes], [gl_cv_func_getopt_gnu=no], [dnl Cross compiling. Assume the worst, even on glibc platforms. gl_cv_func_getopt_gnu="guessing no" ]) case $gl_had_POSIXLY_CORRECT in exported) ;; yes) AS_UNSET([POSIXLY_CORRECT]); POSIXLY_CORRECT=1 ;; *) AS_UNSET([POSIXLY_CORRECT]) ;; esac ]) if test "$gl_cv_func_getopt_gnu" != yes; then gl_replace_getopt=yes else AC_CACHE_CHECK([for working GNU getopt_long function], [gl_cv_func_getopt_long_gnu], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include #include ]], [[static const struct option long_options[] = { { "xtremely-",no_argument, NULL, 1003 }, { "xtra", no_argument, NULL, 1001 }, { "xtreme", no_argument, NULL, 1002 }, { "xtremely", no_argument, NULL, 1003 }, { NULL, 0, NULL, 0 } }; /* This code fails on OpenBSD 5.0. */ { static char program[] = "program"; static char xtremel[] = "--xtremel"; char *argv[] = { program, xtremel, NULL }; int option_index; optind = 1; opterr = 0; if (getopt_long (2, argv, "", long_options, &option_index) != 1003) return 1; } return 0; ]])], [gl_cv_func_getopt_long_gnu=yes], [gl_cv_func_getopt_long_gnu=no], [dnl Cross compiling. Guess no on OpenBSD, yes otherwise. case "$host_os" in openbsd*) gl_cv_func_getopt_long_gnu="guessing no";; *) gl_cv_func_getopt_long_gnu="guessing yes";; esac ]) ]) case "$gl_cv_func_getopt_long_gnu" in *yes) ;; *) gl_replace_getopt=yes ;; esac fi fi ]) AC_DEFUN([gl_GETOPT_SUBSTITUTE_HEADER], [ GETOPT_H=getopt.h AC_DEFINE([__GETOPT_PREFIX], [[rpl_]], [Define to rpl_ if the getopt replacement functions and variables should be used.]) AC_SUBST([GETOPT_H]) ]) # Prerequisites of lib/getopt*. AC_DEFUN([gl_PREREQ_GETOPT], [ AC_CHECK_DECLS_ONCE([getenv]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/getdtablesize.m40000644000175000017500000000324513004436754017245 00000000000000# getdtablesize.m4 serial 6 dnl Copyright (C) 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_GETDTABLESIZE], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) AC_CHECK_FUNCS_ONCE([getdtablesize]) AC_CHECK_DECLS_ONCE([getdtablesize]) if test $ac_cv_func_getdtablesize = yes && test $ac_cv_have_decl_getdtablesize = yes; then # Cygwin 1.7.25 automatically increases the RLIMIT_NOFILE soft limit # up to an unchangeable hard limit; all other platforms correctly # require setrlimit before getdtablesize() can report a larger value. AC_CACHE_CHECK([whether getdtablesize works], [gl_cv_func_getdtablesize_works], [AC_RUN_IFELSE([ AC_LANG_PROGRAM([[#include ]], [int size = getdtablesize(); if (dup2 (0, getdtablesize()) != -1) return 1; if (size != getdtablesize()) return 2; ])], [gl_cv_func_getdtablesize_works=yes], [gl_cv_func_getdtablesize_works=no], [case "$host_os" in cygwin*) # on cygwin 1.5.25, getdtablesize() automatically grows gl_cv_func_getdtablesize_works="guessing no" ;; *) gl_cv_func_getdtablesize_works="guessing yes" ;; esac]) ]) case "$gl_cv_func_getdtablesize_works" in *yes) ;; *) REPLACE_GETDTABLESIZE=1 ;; esac else HAVE_GETDTABLESIZE=0 fi ]) # Prerequisites of lib/getdtablesize.c. AC_DEFUN([gl_PREREQ_GETDTABLESIZE], [:]) gnuastro-0.2.33-8a3b/bootstrapped/m4/getcwd.m40000644000175000017500000001166413004436754015700 00000000000000# getcwd.m4 - check for working getcwd that is compatible with glibc # Copyright (C) 2001, 2003-2007, 2009-2016 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # Written by Paul Eggert. # serial 13 AC_DEFUN([gl_FUNC_GETCWD_NULL], [ AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CHECK_HEADERS_ONCE([unistd.h]) AC_CACHE_CHECK([whether getcwd (NULL, 0) allocates memory for result], [gl_cv_func_getcwd_null], [AC_RUN_IFELSE([AC_LANG_PROGRAM([[ # include # if HAVE_UNISTD_H # include # else /* on Windows with MSVC */ # include # endif # ifndef getcwd char *getcwd (); # endif ]], [[ #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* mingw cwd does not start with '/', but getcwd does allocate. However, mingw fails to honor non-zero size. */ #else if (chdir ("/") != 0) return 1; else { char *f = getcwd (NULL, 0); if (! f) return 2; if (f[0] != '/') return 3; if (f[1] != '\0') return 4; free (f); return 0; } #endif ]])], [gl_cv_func_getcwd_null=yes], [gl_cv_func_getcwd_null=no], [[case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_getcwd_null="guessing yes";; # Guess yes on Cygwin. cygwin*) gl_cv_func_getcwd_null="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_getcwd_null="guessing no";; esac ]])]) ]) AC_DEFUN([gl_FUNC_GETCWD_SIGNATURE], [ AC_CACHE_CHECK([for getcwd with POSIX signature], [gl_cv_func_getcwd_posix_signature], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[extern #ifdef __cplusplus "C" #endif char *getcwd (char *, size_t); ]]) ], [gl_cv_func_getcwd_posix_signature=yes], [gl_cv_func_getcwd_posix_signature=no]) ]) ]) dnl Guarantee that getcwd will malloc with a NULL first argument. Assumes dnl that either the system getcwd is robust, or that calling code is okay dnl with spurious failures when run from a directory with an absolute name dnl larger than 4k bytes. dnl dnl Assumes that getcwd exists; if you are worried about obsolete dnl platforms that lacked getcwd(), then you need to use the GPL module. AC_DEFUN([gl_FUNC_GETCWD_LGPL], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([gl_FUNC_GETCWD_NULL]) AC_REQUIRE([gl_FUNC_GETCWD_SIGNATURE]) case $gl_cv_func_getcwd_null,$gl_cv_func_getcwd_posix_signature in *yes,yes) ;; *) dnl Minimal replacement lib/getcwd-lgpl.c. REPLACE_GETCWD=1 ;; esac ]) dnl Check for all known getcwd bugs; useful for a program likely to be dnl executed from an arbitrary location. AC_DEFUN([gl_FUNC_GETCWD], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([gl_FUNC_GETCWD_NULL]) AC_REQUIRE([gl_FUNC_GETCWD_SIGNATURE]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles gl_abort_bug=no case "$host_os" in mingw*) gl_cv_func_getcwd_path_max=yes ;; *) gl_FUNC_GETCWD_PATH_MAX case "$gl_cv_func_getcwd_null" in *yes) gl_FUNC_GETCWD_ABORT_BUG([gl_abort_bug=yes]) ;; esac ;; esac dnl Define HAVE_MINIMALLY_WORKING_GETCWD and HAVE_PARTLY_WORKING_GETCWD dnl if appropriate. case "$gl_cv_func_getcwd_path_max" in "no"|"no, it has the AIX bug") ;; *) AC_DEFINE([HAVE_MINIMALLY_WORKING_GETCWD], [1], [Define to 1 if getcwd minimally works, that is, its result can be trusted when it succeeds.]) ;; esac case "$gl_cv_func_getcwd_path_max" in "no, but it is partly working") AC_DEFINE([HAVE_PARTLY_WORKING_GETCWD], [1], [Define to 1 if getcwd works, except it sometimes fails when it shouldn't, setting errno to ERANGE, ENAMETOOLONG, or ENOENT.]) ;; "yes, but with shorter paths") AC_DEFINE([HAVE_GETCWD_SHORTER], [1], [Define to 1 if getcwd works, but with shorter paths than is generally tested with the replacement.]) ;; esac if { case "$gl_cv_func_getcwd_null" in *yes) false;; *) true;; esac; } \ || test $gl_cv_func_getcwd_posix_signature != yes \ || { case "$gl_cv_func_getcwd_path_max" in *yes*) false;; *) true;; esac; } \ || test $gl_abort_bug = yes; then REPLACE_GETCWD=1 fi ]) # Prerequisites of lib/getcwd.c, when full replacement is in effect. AC_DEFUN([gl_PREREQ_GETCWD], [ AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([gl_CHECK_TYPE_STRUCT_DIRENT_D_INO]) : ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/fstat.m40000644000175000017500000000164613004436754015543 00000000000000# fstat.m4 serial 4 dnl Copyright (C) 2011-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_FSTAT], [ AC_REQUIRE([gl_SYS_STAT_H_DEFAULTS]) AC_REQUIRE([gl_MSVC_INVAL]) if test $HAVE_MSVC_INVALID_PARAMETER_HANDLER = 1; then REPLACE_FSTAT=1 fi AC_REQUIRE([gl_HEADER_SYS_STAT_H]) if test $WINDOWS_64_BIT_ST_SIZE = 1; then REPLACE_FSTAT=1 fi dnl Replace fstat() for supporting the gnulib-defined open() on directories. m4_ifdef([gl_FUNC_FCHDIR], [ gl_TEST_FCHDIR if test $HAVE_FCHDIR = 0; then case "$gl_cv_func_open_directory_works" in *yes) ;; *) REPLACE_FSTAT=1 ;; esac fi ]) ]) # Prerequisites of lib/fstat.c. AC_DEFUN([gl_PREREQ_FSTAT], [:]) gnuastro-0.2.33-8a3b/bootstrapped/m4/fpieee.m40000644000175000017500000000440513004436754015653 00000000000000# fpieee.m4 serial 2 -*- coding: utf-8 -*- dnl Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl IEEE 754 standardized three items: dnl - The formats of single-float and double-float - nowadays commonly dnl available as 'float' and 'double' in C and C++. dnl No autoconf test needed. dnl - The overflow and division by zero behaviour: The result are values dnl '±Inf' and 'NaN', rather than exceptions as it was before. dnl This file provides an autoconf macro for ensuring this behaviour of dnl floating-point operations. dnl - A set of conditions (overflow, underflow, inexact, etc.) which can dnl be configured to trigger an exception. dnl This cannot be done in a portable way: it depends on the compiler, dnl libc, kernel, and CPU. No autoconf macro is provided for this. dnl Ensure non-trapping behaviour of floating-point overflow and dnl floating-point division by zero. dnl (For integer overflow, see gcc's -ftrapv option; for integer division by dnl zero, see the autoconf macro in intdiv0.m4.) AC_DEFUN([gl_FP_IEEE], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) # IEEE behaviour is the default on all CPUs except Alpha and SH # (according to the test results of Bruno Haible's ieeefp/fenv_default.m4 # and the GCC 4.1.2 manual). case "$host_cpu" in alpha*) # On Alpha systems, a compiler option provides the behaviour. # See the ieee(3) manual page, also available at # if test -n "$GCC"; then # GCC has the option -mieee. # For full IEEE compliance (rarely needed), use option -mieee-with-inexact. CPPFLAGS="$CPPFLAGS -mieee" else # Compaq (ex-DEC) C has the option -ieee, equivalent to -ieee_with_no_inexact. # For full IEEE compliance (rarely needed), use option -ieee_with_inexact. CPPFLAGS="$CPPFLAGS -ieee" fi ;; sh*) if test -n "$GCC"; then # GCC has the option -mieee. CPPFLAGS="$CPPFLAGS -mieee" fi ;; esac ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/float_h.m40000644000175000017500000000466313004436754016040 00000000000000# float_h.m4 serial 9 dnl Copyright (C) 2007, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FLOAT_H], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) FLOAT_H= REPLACE_FLOAT_LDBL=0 case "$host_os" in aix* | beos* | openbsd* | mirbsd* | irix*) FLOAT_H=float.h ;; freebsd*) case "$host_cpu" in changequote(,)dnl i[34567]86 ) changequote([,])dnl FLOAT_H=float.h ;; x86_64 ) # On x86_64 systems, the C compiler may still be generating # 32-bit code. AC_EGREP_CPP([yes], [#if defined __LP64__ || defined __x86_64__ || defined __amd64__ yes #endif], [], [FLOAT_H=float.h]) ;; esac ;; linux*) case "$host_cpu" in powerpc*) FLOAT_H=float.h ;; esac ;; esac case "$host_os" in aix* | freebsd* | linux*) if test -n "$FLOAT_H"; then REPLACE_FLOAT_LDBL=1 fi ;; esac dnl Test against glibc-2.7 Linux/SPARC64 bug. REPLACE_ITOLD=0 AC_CACHE_CHECK([whether conversion from 'int' to 'long double' works], [gl_cv_func_itold_works], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ int i = -1; volatile long double ld; int main () { ld += i * 1.0L; if (ld > 0) return 1; return 0; }]])], [gl_cv_func_itold_works=yes], [gl_cv_func_itold_works=no], [case "$host" in sparc*-*-linux*) AC_EGREP_CPP([yes], [#if defined __LP64__ || defined __arch64__ yes #endif], [gl_cv_func_itold_works="guessing no"], [gl_cv_func_itold_works="guessing yes"]) ;; *) gl_cv_func_itold_works="guessing yes" ;; esac ]) ]) case "$gl_cv_func_itold_works" in *no) REPLACE_ITOLD=1 dnl We add the workaround to but also to , dnl to increase the chances that the fix function gets pulled in. FLOAT_H=float.h ;; esac if test -n "$FLOAT_H"; then gl_NEXT_HEADERS([float.h]) fi AC_SUBST([FLOAT_H]) AM_CONDITIONAL([GL_GENERATE_FLOAT_H], [test -n "$FLOAT_H"]) AC_SUBST([REPLACE_ITOLD]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/flexmember.m40000644000175000017500000000324313004436754016543 00000000000000# serial 4 # Check for flexible array member support. # Copyright (C) 2006, 2009-2016 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # Written by Paul Eggert. AC_DEFUN([AC_C_FLEXIBLE_ARRAY_MEMBER], [ AC_CACHE_CHECK([for flexible array member], ac_cv_c_flexmember, [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include #include #include struct s { int n; double d[]; };]], [[int m = getchar (); size_t nbytes = offsetof (struct s, d) + m * sizeof (double); nbytes += sizeof (struct s) - 1; nbytes -= nbytes % sizeof (struct s); struct s *p = malloc (nbytes); p->d[0] = 0.0; return p->d != (double *) NULL;]])], [ac_cv_c_flexmember=yes], [ac_cv_c_flexmember=no])]) if test $ac_cv_c_flexmember = yes; then AC_DEFINE([FLEXIBLE_ARRAY_MEMBER], [], [Define to nothing if C supports flexible array members, and to 1 if it does not. That way, with a declaration like 'struct s { int n; double d@<:@FLEXIBLE_ARRAY_MEMBER@:>@; };', the struct hack can be used with pre-C99 compilers. When computing the size of such an object, don't use 'sizeof (struct s)' as it overestimates the size. Use 'offsetof (struct s, d)' instead. Don't use 'offsetof (struct s, d@<:@0@:>@)', as this doesn't work with MSVC and with C++ compilers.]) else AC_DEFINE([FLEXIBLE_ARRAY_MEMBER], [1]) fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/fdopen.m40000644000175000017500000000246113004436754015671 00000000000000# fdopen.m4 serial 3 dnl Copyright (C) 2011-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_FDOPEN], [ AC_REQUIRE([gl_STDIO_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_MSVC_INVAL]) if test $HAVE_MSVC_INVALID_PARAMETER_HANDLER = 1; then REPLACE_FDOPEN=1 else dnl Test whether fdopen() sets errno when it fails due to a bad fd argument. AC_CACHE_CHECK([whether fdopen sets errno], [gl_cv_func_fdopen_works], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include int main (void) { FILE *fp; errno = 0; fp = fdopen (-1, "r"); if (fp == NULL && errno == 0) return 1; return 0; }]])], [gl_cv_func_fdopen_works=yes], [gl_cv_func_fdopen_works=no], [case "$host_os" in mingw*) gl_cv_func_fdopen_works="guessing no" ;; *) gl_cv_func_fdopen_works="guessing yes" ;; esac ]) ]) case "$gl_cv_func_fdopen_works" in *no) REPLACE_FDOPEN=1 ;; esac fi ]) dnl Prerequisites of lib/fdopen.c. AC_DEFUN([gl_PREREQ_FDOPEN], []) gnuastro-0.2.33-8a3b/bootstrapped/m4/fcntl_h.m40000644000175000017500000000327113004436754016033 00000000000000# serial 15 # Configure fcntl.h. dnl Copyright (C) 2006-2007, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Written by Paul Eggert. AC_DEFUN([gl_FCNTL_H], [ AC_REQUIRE([gl_FCNTL_H_DEFAULTS]) AC_REQUIRE([gl_FCNTL_O_FLAGS]) gl_NEXT_HEADERS([fcntl.h]) dnl Ensure the type pid_t gets defined. AC_REQUIRE([AC_TYPE_PID_T]) dnl Ensure the type mode_t gets defined. AC_REQUIRE([AC_TYPE_MODE_T]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use, if it is not common dnl enough to be declared everywhere. gl_WARN_ON_USE_PREPARE([[#include ]], [fcntl openat]) ]) AC_DEFUN([gl_FCNTL_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_FCNTL_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_FCNTL_H_DEFAULTS], [ GNULIB_FCNTL=0; AC_SUBST([GNULIB_FCNTL]) GNULIB_NONBLOCKING=0; AC_SUBST([GNULIB_NONBLOCKING]) GNULIB_OPEN=0; AC_SUBST([GNULIB_OPEN]) GNULIB_OPENAT=0; AC_SUBST([GNULIB_OPENAT]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_FCNTL=1; AC_SUBST([HAVE_FCNTL]) HAVE_OPENAT=1; AC_SUBST([HAVE_OPENAT]) REPLACE_FCNTL=0; AC_SUBST([REPLACE_FCNTL]) REPLACE_OPEN=0; AC_SUBST([REPLACE_OPEN]) REPLACE_OPENAT=0; AC_SUBST([REPLACE_OPENAT]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/fcntl-o.m40000644000175000017500000001107413004436754015760 00000000000000# fcntl-o.m4 serial 4 dnl Copyright (C) 2006, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Written by Paul Eggert. # Test whether the flags O_NOATIME and O_NOFOLLOW actually work. # Define HAVE_WORKING_O_NOATIME to 1 if O_NOATIME works, or to 0 otherwise. # Define HAVE_WORKING_O_NOFOLLOW to 1 if O_NOFOLLOW works, or to 0 otherwise. AC_DEFUN([gl_FCNTL_O_FLAGS], [ dnl Persuade glibc to define O_NOATIME and O_NOFOLLOW. dnl AC_USE_SYSTEM_EXTENSIONS was introduced in autoconf 2.60 and obsoletes dnl AC_GNU_SOURCE. m4_ifdef([AC_USE_SYSTEM_EXTENSIONS], [AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS])], [AC_REQUIRE([AC_GNU_SOURCE])]) AC_CHECK_HEADERS_ONCE([unistd.h]) AC_CHECK_FUNCS_ONCE([symlink]) AC_CACHE_CHECK([for working fcntl.h], [gl_cv_header_working_fcntl_h], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include #if HAVE_UNISTD_H # include #else /* on Windows with MSVC */ # include # include # defined sleep(n) _sleep ((n) * 1000) #endif #include #ifndef O_NOATIME #define O_NOATIME 0 #endif #ifndef O_NOFOLLOW #define O_NOFOLLOW 0 #endif static int const constants[] = { O_CREAT, O_EXCL, O_NOCTTY, O_TRUNC, O_APPEND, O_NONBLOCK, O_SYNC, O_ACCMODE, O_RDONLY, O_RDWR, O_WRONLY }; ]], [[ int result = !constants; #if HAVE_SYMLINK { static char const sym[] = "conftest.sym"; if (symlink ("/dev/null", sym) != 0) result |= 2; else { int fd = open (sym, O_WRONLY | O_NOFOLLOW | O_CREAT, 0); if (fd >= 0) { close (fd); result |= 4; } } if (unlink (sym) != 0 || symlink (".", sym) != 0) result |= 2; else { int fd = open (sym, O_RDONLY | O_NOFOLLOW); if (fd >= 0) { close (fd); result |= 4; } } unlink (sym); } #endif { static char const file[] = "confdefs.h"; int fd = open (file, O_RDONLY | O_NOATIME); if (fd < 0) result |= 8; else { struct stat st0; if (fstat (fd, &st0) != 0) result |= 16; else { char c; sleep (1); if (read (fd, &c, 1) != 1) result |= 24; else { if (close (fd) != 0) result |= 32; else { struct stat st1; if (stat (file, &st1) != 0) result |= 40; else if (st0.st_atime != st1.st_atime) result |= 64; } } } } } return result;]])], [gl_cv_header_working_fcntl_h=yes], [case $? in #( 4) gl_cv_header_working_fcntl_h='no (bad O_NOFOLLOW)';; #( 64) gl_cv_header_working_fcntl_h='no (bad O_NOATIME)';; #( 68) gl_cv_header_working_fcntl_h='no (bad O_NOATIME, O_NOFOLLOW)';; #( *) gl_cv_header_working_fcntl_h='no';; esac], [gl_cv_header_working_fcntl_h=cross-compiling])]) case $gl_cv_header_working_fcntl_h in #( *O_NOATIME* | no | cross-compiling) ac_val=0;; #( *) ac_val=1;; esac AC_DEFINE_UNQUOTED([HAVE_WORKING_O_NOATIME], [$ac_val], [Define to 1 if O_NOATIME works.]) case $gl_cv_header_working_fcntl_h in #( *O_NOFOLLOW* | no | cross-compiling) ac_val=0;; #( *) ac_val=1;; esac AC_DEFINE_UNQUOTED([HAVE_WORKING_O_NOFOLLOW], [$ac_val], [Define to 1 if O_NOFOLLOW works.]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/extern-inline.m40000644000175000017500000001042013004436754017171 00000000000000dnl 'extern inline' a la ISO C99. dnl Copyright 2012-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_EXTERN_INLINE], [ AH_VERBATIM([extern_inline], [/* Please see the Gnulib manual for how to use these macros. Suppress extern inline with HP-UX cc, as it appears to be broken; see . Suppress extern inline with Sun C in standards-conformance mode, as it mishandles inline functions that call each other. E.g., for 'inline void f (void) { } inline void g (void) { f (); }', c99 incorrectly complains 'reference to static identifier "f" in extern inline function'. This bug was observed with Sun C 5.12 SunOS_i386 2011/11/16. Suppress extern inline (with or without __attribute__ ((__gnu_inline__))) on configurations that mistakenly use 'static inline' to implement functions or macros in standard C headers like . For example, if isdigit is mistakenly implemented via a static inline function, a program containing an extern inline function that calls isdigit may not work since the C standard prohibits extern inline functions from calling static functions. This bug is known to occur on: OS X 10.8 and earlier; see: http://lists.gnu.org/archive/html/bug-gnulib/2012-12/msg00023.html DragonFly; see http://muscles.dragonflybsd.org/bulk/bleeding-edge-potential/latest-per-pkg/ah-tty-0.3.12.log FreeBSD; see: http://lists.gnu.org/archive/html/bug-gnulib/2014-07/msg00104.html OS X 10.9 has a macro __header_inline indicating the bug is fixed for C and for clang but remains for g++; see . Assume DragonFly and FreeBSD will be similar. */ #if (((defined __APPLE__ && defined __MACH__) \ || defined __DragonFly__ || defined __FreeBSD__) \ && (defined __header_inline \ ? (defined __cplusplus && defined __GNUC_STDC_INLINE__ \ && ! defined __clang__) \ : ((! defined _DONT_USE_CTYPE_INLINE_ \ && (defined __GNUC__ || defined __cplusplus)) \ || (defined _FORTIFY_SOURCE && 0 < _FORTIFY_SOURCE \ && defined __GNUC__ && ! defined __cplusplus)))) # define _GL_EXTERN_INLINE_STDHEADER_BUG #endif #if ((__GNUC__ \ ? defined __GNUC_STDC_INLINE__ && __GNUC_STDC_INLINE__ \ : (199901L <= __STDC_VERSION__ \ && !defined __HP_cc \ && !defined __PGI \ && !(defined __SUNPRO_C && __STDC__))) \ && !defined _GL_EXTERN_INLINE_STDHEADER_BUG) # define _GL_INLINE inline # define _GL_EXTERN_INLINE extern inline # define _GL_EXTERN_INLINE_IN_USE #elif (2 < __GNUC__ + (7 <= __GNUC_MINOR__) && !defined __STRICT_ANSI__ \ && !defined _GL_EXTERN_INLINE_STDHEADER_BUG) # if defined __GNUC_GNU_INLINE__ && __GNUC_GNU_INLINE__ /* __gnu_inline__ suppresses a GCC 4.2 diagnostic. */ # define _GL_INLINE extern inline __attribute__ ((__gnu_inline__)) # else # define _GL_INLINE extern inline # endif # define _GL_EXTERN_INLINE extern # define _GL_EXTERN_INLINE_IN_USE #else # define _GL_INLINE static _GL_UNUSED # define _GL_EXTERN_INLINE static _GL_UNUSED #endif /* In GCC 4.6 (inclusive) to 5.1 (exclusive), suppress bogus "no previous prototype for 'FOO'" and "no previous declaration for 'FOO'" diagnostics, when FOO is an inline function in the header; see and . */ #if __GNUC__ == 4 && 6 <= __GNUC_MINOR__ # if defined __GNUC_STDC_INLINE__ && __GNUC_STDC_INLINE__ # define _GL_INLINE_HEADER_CONST_PRAGMA # else # define _GL_INLINE_HEADER_CONST_PRAGMA \ _Pragma ("GCC diagnostic ignored \"-Wsuggest-attribute=const\"") # endif # define _GL_INLINE_HEADER_BEGIN \ _Pragma ("GCC diagnostic push") \ _Pragma ("GCC diagnostic ignored \"-Wmissing-prototypes\"") \ _Pragma ("GCC diagnostic ignored \"-Wmissing-declarations\"") \ _GL_INLINE_HEADER_CONST_PRAGMA # define _GL_INLINE_HEADER_END \ _Pragma ("GCC diagnostic pop") #else # define _GL_INLINE_HEADER_BEGIN # define _GL_INLINE_HEADER_END #endif]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/extensions.m40000644000175000017500000001476513004436754016627 00000000000000# serial 15 -*- Autoconf -*- # Enable extensions on systems that normally disable them. # Copyright (C) 2003, 2006-2016 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # This definition of AC_USE_SYSTEM_EXTENSIONS is stolen from git # Autoconf. Perhaps we can remove this once we can assume Autoconf # 2.70 or later everywhere, but since Autoconf mutates rapidly # enough in this area it's likely we'll need to redefine # AC_USE_SYSTEM_EXTENSIONS for quite some time. # If autoconf reports a warning # warning: AC_COMPILE_IFELSE was called before AC_USE_SYSTEM_EXTENSIONS # or warning: AC_RUN_IFELSE was called before AC_USE_SYSTEM_EXTENSIONS # the fix is # 1) to ensure that AC_USE_SYSTEM_EXTENSIONS is never directly invoked # but always AC_REQUIREd, # 2) to ensure that for each occurrence of # AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) # or # AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) # the corresponding gnulib module description has 'extensions' among # its dependencies. This will ensure that the gl_USE_SYSTEM_EXTENSIONS # invocation occurs in gl_EARLY, not in gl_INIT. # AC_USE_SYSTEM_EXTENSIONS # ------------------------ # Enable extensions on systems that normally disable them, # typically due to standards-conformance issues. # # Remember that #undef in AH_VERBATIM gets replaced with #define by # AC_DEFINE. The goal here is to define all known feature-enabling # macros, then, if reports of conflicts are made, disable macros that # cause problems on some platforms (such as __EXTENSIONS__). AC_DEFUN_ONCE([AC_USE_SYSTEM_EXTENSIONS], [AC_BEFORE([$0], [AC_COMPILE_IFELSE])dnl AC_BEFORE([$0], [AC_RUN_IFELSE])dnl AC_CHECK_HEADER([minix/config.h], [MINIX=yes], [MINIX=]) if test "$MINIX" = yes; then AC_DEFINE([_POSIX_SOURCE], [1], [Define to 1 if you need to in order for 'stat' and other things to work.]) AC_DEFINE([_POSIX_1_SOURCE], [2], [Define to 2 if the system does not provide POSIX.1 features except with this defined.]) AC_DEFINE([_MINIX], [1], [Define to 1 if on MINIX.]) AC_DEFINE([_NETBSD_SOURCE], [1], [Define to 1 to make NetBSD features available. MINIX 3 needs this.]) fi dnl Use a different key than __EXTENSIONS__, as that name broke existing dnl configure.ac when using autoheader 2.62. AH_VERBATIM([USE_SYSTEM_EXTENSIONS], [/* Enable extensions on AIX 3, Interix. */ #ifndef _ALL_SOURCE # undef _ALL_SOURCE #endif /* Enable general extensions on macOS. */ #ifndef _DARWIN_C_SOURCE # undef _DARWIN_C_SOURCE #endif /* Enable GNU extensions on systems that have them. */ #ifndef _GNU_SOURCE # undef _GNU_SOURCE #endif /* Enable threading extensions on Solaris. */ #ifndef _POSIX_PTHREAD_SEMANTICS # undef _POSIX_PTHREAD_SEMANTICS #endif /* Enable extensions specified by ISO/IEC TS 18661-5:2014. */ #ifndef __STDC_WANT_IEC_60559_ATTRIBS_EXT__ # undef __STDC_WANT_IEC_60559_ATTRIBS_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-1:2014. */ #ifndef __STDC_WANT_IEC_60559_BFP_EXT__ # undef __STDC_WANT_IEC_60559_BFP_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-2:2015. */ #ifndef __STDC_WANT_IEC_60559_DFP_EXT__ # undef __STDC_WANT_IEC_60559_DFP_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-4:2015. */ #ifndef __STDC_WANT_IEC_60559_FUNCS_EXT__ # undef __STDC_WANT_IEC_60559_FUNCS_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-3:2015. */ #ifndef __STDC_WANT_IEC_60559_TYPES_EXT__ # undef __STDC_WANT_IEC_60559_TYPES_EXT__ #endif /* Enable extensions specified by ISO/IEC TR 24731-2:2010. */ #ifndef __STDC_WANT_LIB_EXT2__ # undef __STDC_WANT_LIB_EXT2__ #endif /* Enable extensions specified by ISO/IEC 24747:2009. */ #ifndef __STDC_WANT_MATH_SPEC_FUNCS__ # undef __STDC_WANT_MATH_SPEC_FUNCS__ #endif /* Enable extensions on HP NonStop. */ #ifndef _TANDEM_SOURCE # undef _TANDEM_SOURCE #endif /* Enable X/Open extensions if necessary. HP-UX 11.11 defines mbstate_t only if _XOPEN_SOURCE is defined to 500, regardless of whether compiling with -Ae or -D_HPUX_SOURCE=1. */ #ifndef _XOPEN_SOURCE # undef _XOPEN_SOURCE #endif /* Enable general extensions on Solaris. */ #ifndef __EXTENSIONS__ # undef __EXTENSIONS__ #endif ]) AC_CACHE_CHECK([whether it is safe to define __EXTENSIONS__], [ac_cv_safe_to_define___extensions__], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[ # define __EXTENSIONS__ 1 ]AC_INCLUDES_DEFAULT])], [ac_cv_safe_to_define___extensions__=yes], [ac_cv_safe_to_define___extensions__=no])]) test $ac_cv_safe_to_define___extensions__ = yes && AC_DEFINE([__EXTENSIONS__]) AC_DEFINE([_ALL_SOURCE]) AC_DEFINE([_DARWIN_C_SOURCE]) AC_DEFINE([_GNU_SOURCE]) AC_DEFINE([_POSIX_PTHREAD_SEMANTICS]) AC_DEFINE([__STDC_WANT_IEC_60559_ATTRIBS_EXT__]) AC_DEFINE([__STDC_WANT_IEC_60559_BFP_EXT__]) AC_DEFINE([__STDC_WANT_IEC_60559_DFP_EXT__]) AC_DEFINE([__STDC_WANT_IEC_60559_FUNCS_EXT__]) AC_DEFINE([__STDC_WANT_IEC_60559_TYPES_EXT__]) AC_DEFINE([__STDC_WANT_LIB_EXT2__]) AC_DEFINE([__STDC_WANT_MATH_SPEC_FUNCS__]) AC_DEFINE([_TANDEM_SOURCE]) AC_CACHE_CHECK([whether _XOPEN_SOURCE should be defined], [ac_cv_should_define__xopen_source], [ac_cv_should_define__xopen_source=no AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[ #include mbstate_t x;]])], [], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[ #define _XOPEN_SOURCE 500 #include mbstate_t x;]])], [ac_cv_should_define__xopen_source=yes])])]) test $ac_cv_should_define__xopen_source = yes && AC_DEFINE([_XOPEN_SOURCE], [500]) ])# AC_USE_SYSTEM_EXTENSIONS # gl_USE_SYSTEM_EXTENSIONS # ------------------------ # Enable extensions on systems that normally disable them, # typically due to standards-conformance issues. AC_DEFUN_ONCE([gl_USE_SYSTEM_EXTENSIONS], [ dnl Require this macro before AC_USE_SYSTEM_EXTENSIONS. dnl gnulib does not need it. But if it gets required by third-party macros dnl after AC_USE_SYSTEM_EXTENSIONS is required, autoconf 2.62..2.63 emit a dnl warning: "AC_COMPILE_IFELSE was called before AC_USE_SYSTEM_EXTENSIONS". dnl Note: We can do this only for one of the macros AC_AIX, AC_GNU_SOURCE, dnl AC_MINIX. If people still use AC_AIX or AC_MINIX, they are out of luck. AC_REQUIRE([AC_GNU_SOURCE]) AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/exponentd.m40000644000175000017500000000755213004436754016430 00000000000000# exponentd.m4 serial 3 dnl Copyright (C) 2007-2008, 2010-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_DOUBLE_EXPONENT_LOCATION], [ AC_CACHE_CHECK([where to find the exponent in a 'double'], [gl_cv_cc_double_expbit0], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include #include #define NWORDS \ ((sizeof (double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { double value; unsigned int word[NWORDS]; } memory_double; static unsigned int ored_words[NWORDS]; static unsigned int anded_words[NWORDS]; static void add_to_ored_words (double x) { memory_double m; size_t i; /* Clear it first, in case sizeof (double) < sizeof (memory_double). */ memset (&m, 0, sizeof (memory_double)); m.value = x; for (i = 0; i < NWORDS; i++) { ored_words[i] |= m.word[i]; anded_words[i] &= m.word[i]; } } int main () { size_t j; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; for (j = 0; j < NWORDS; j++) anded_words[j] = ~ (unsigned int) 0; add_to_ored_words (0.25); add_to_ored_words (0.5); add_to_ored_words (1.0); add_to_ored_words (2.0); add_to_ored_words (4.0); /* Remove bits that are common (e.g. if representation of the first mantissa bit is explicit). */ for (j = 0; j < NWORDS; j++) ored_words[j] &= ~anded_words[j]; /* Now find the nonzero word. */ for (j = 0; j < NWORDS; j++) if (ored_words[j] != 0) break; if (j < NWORDS) { size_t i; for (i = j + 1; i < NWORDS; i++) if (ored_words[i] != 0) { fprintf (fp, "unknown"); return (fclose (fp) != 0); } for (i = 0; ; i++) if ((ored_words[j] >> i) & 1) { fprintf (fp, "word %d bit %d", (int) j, (int) i); return (fclose (fp) != 0); } } fprintf (fp, "unknown"); return (fclose (fp) != 0); } ]])], [gl_cv_cc_double_expbit0=`cat conftest.out`], [gl_cv_cc_double_expbit0="unknown"], [ dnl On ARM, there are two 'double' floating-point formats, used by dnl different sets of instructions: The older FPA instructions assume dnl that they are stored in big-endian word order, while the words dnl (like integer types) are stored in little-endian byte order. dnl The newer VFP instructions assume little-endian order dnl consistently. AC_EGREP_CPP([mixed_endianness], [ #if defined arm || defined __arm || defined __arm__ mixed_endianness #endif ], [gl_cv_cc_double_expbit0="unknown"], [ pushdef([AC_MSG_CHECKING],[:])dnl pushdef([AC_MSG_RESULT],[:])dnl pushdef([AC_MSG_RESULT_UNQUOTED],[:])dnl AC_C_BIGENDIAN( [gl_cv_cc_double_expbit0="word 0 bit 20"], [gl_cv_cc_double_expbit0="word 1 bit 20"], [gl_cv_cc_double_expbit0="unknown"]) popdef([AC_MSG_RESULT_UNQUOTED])dnl popdef([AC_MSG_RESULT])dnl popdef([AC_MSG_CHECKING])dnl ]) ]) rm -f conftest.out ]) case "$gl_cv_cc_double_expbit0" in word*bit*) word=`echo "$gl_cv_cc_double_expbit0" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$gl_cv_cc_double_expbit0" | sed -e 's/word.*bit //'` AC_DEFINE_UNQUOTED([DBL_EXPBIT0_WORD], [$word], [Define as the word index where to find the exponent of 'double'.]) AC_DEFINE_UNQUOTED([DBL_EXPBIT0_BIT], [$bit], [Define as the bit index in the word where to find bit 0 of the exponent of 'double'.]) ;; esac ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/error.m40000644000175000017500000000151013004436754015541 00000000000000#serial 14 # Copyright (C) 1996-1998, 2001-2004, 2009-2016 Free Software Foundation, Inc. # # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_ERROR], [ dnl We don't use AC_FUNC_ERROR_AT_LINE any more, because it is no longer dnl maintained in Autoconf and because it invokes AC_LIBOBJ. AC_CACHE_CHECK([for error_at_line], [ac_cv_lib_error_at_line], [AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[error_at_line (0, 0, "", 0, "an error occurred");]])], [ac_cv_lib_error_at_line=yes], [ac_cv_lib_error_at_line=no])]) ]) # Prerequisites of lib/error.c. AC_DEFUN([gl_PREREQ_ERROR], [ AC_REQUIRE([AC_FUNC_STRERROR_R]) : ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/errno_h.m40000644000175000017500000000623413004436754016054 00000000000000# errno_h.m4 serial 12 dnl Copyright (C) 2004, 2006, 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN_ONCE([gl_HEADER_ERRNO_H], [ AC_REQUIRE([AC_PROG_CC]) AC_CACHE_CHECK([for complete errno.h], [gl_cv_header_errno_h_complete], [ AC_EGREP_CPP([booboo],[ #include #if !defined ETXTBSY booboo #endif #if !defined ENOMSG booboo #endif #if !defined EIDRM booboo #endif #if !defined ENOLINK booboo #endif #if !defined EPROTO booboo #endif #if !defined EMULTIHOP booboo #endif #if !defined EBADMSG booboo #endif #if !defined EOVERFLOW booboo #endif #if !defined ENOTSUP booboo #endif #if !defined ENETRESET booboo #endif #if !defined ECONNABORTED booboo #endif #if !defined ESTALE booboo #endif #if !defined EDQUOT booboo #endif #if !defined ECANCELED booboo #endif #if !defined EOWNERDEAD booboo #endif #if !defined ENOTRECOVERABLE booboo #endif #if !defined EILSEQ booboo #endif ], [gl_cv_header_errno_h_complete=no], [gl_cv_header_errno_h_complete=yes]) ]) if test $gl_cv_header_errno_h_complete = yes; then ERRNO_H='' else gl_NEXT_HEADERS([errno.h]) ERRNO_H='errno.h' fi AC_SUBST([ERRNO_H]) AM_CONDITIONAL([GL_GENERATE_ERRNO_H], [test -n "$ERRNO_H"]) gl_REPLACE_ERRNO_VALUE([EMULTIHOP]) gl_REPLACE_ERRNO_VALUE([ENOLINK]) gl_REPLACE_ERRNO_VALUE([EOVERFLOW]) ]) # Assuming $1 = EOVERFLOW. # The EOVERFLOW errno value ought to be defined in , according to # POSIX. But some systems (like OpenBSD 4.0 or AIX 3) don't define it, and # some systems (like OSF/1) define it when _XOPEN_SOURCE_EXTENDED is defined. # Check for the value of EOVERFLOW. # Set the variables EOVERFLOW_HIDDEN and EOVERFLOW_VALUE. AC_DEFUN([gl_REPLACE_ERRNO_VALUE], [ if test -n "$ERRNO_H"; then AC_CACHE_CHECK([for ]$1[ value], [gl_cv_header_errno_h_]$1, [ AC_EGREP_CPP([yes],[ #include #ifdef ]$1[ yes #endif ], [gl_cv_header_errno_h_]$1[=yes], [gl_cv_header_errno_h_]$1[=no]) if test $gl_cv_header_errno_h_]$1[ = no; then AC_EGREP_CPP([yes],[ #define _XOPEN_SOURCE_EXTENDED 1 #include #ifdef ]$1[ yes #endif ], [gl_cv_header_errno_h_]$1[=hidden]) if test $gl_cv_header_errno_h_]$1[ = hidden; then dnl The macro exists but is hidden. dnl Define it to the same value. AC_COMPUTE_INT([gl_cv_header_errno_h_]$1, $1, [ #define _XOPEN_SOURCE_EXTENDED 1 #include /* The following two lines are a workaround against an autoconf-2.52 bug. */ #include #include ]) fi fi ]) case $gl_cv_header_errno_h_]$1[ in yes | no) ]$1[_HIDDEN=0; ]$1[_VALUE= ;; *) ]$1[_HIDDEN=1; ]$1[_VALUE="$gl_cv_header_errno_h_]$1[" ;; esac AC_SUBST($1[_HIDDEN]) AC_SUBST($1[_VALUE]) fi ]) dnl Autoconf >= 2.61 has AC_COMPUTE_INT built-in. dnl Remove this when we can assume autoconf >= 2.61. m4_ifdef([AC_COMPUTE_INT], [], [ AC_DEFUN([AC_COMPUTE_INT], [_AC_COMPUTE_INT([$2],[$1],[$3],[$4])]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/environ.m40000644000175000017500000000261613004436754016100 00000000000000# environ.m4 serial 6 dnl Copyright (C) 2001-2004, 2006-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN_ONCE([gl_ENVIRON], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) dnl Persuade glibc to declare environ. AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) AC_CHECK_HEADERS_ONCE([unistd.h]) gt_CHECK_VAR_DECL( [#if HAVE_UNISTD_H #include #endif /* mingw, BeOS, Haiku declare environ in , not in . */ #include ], [environ]) if test $gt_cv_var_environ_declaration != yes; then HAVE_DECL_ENVIRON=0 fi ]) # Check if a variable is properly declared. # gt_CHECK_VAR_DECL(includes,variable) AC_DEFUN([gt_CHECK_VAR_DECL], [ define([gt_cv_var], [gt_cv_var_]$2[_declaration]) AC_MSG_CHECKING([if $2 is properly declared]) AC_CACHE_VAL([gt_cv_var], [ AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[$1 extern struct { int foo; } $2;]], [[$2.foo = 1;]])], [gt_cv_var=no], [gt_cv_var=yes])]) AC_MSG_RESULT([$gt_cv_var]) if test $gt_cv_var = yes; then AC_DEFINE([HAVE_]m4_translit($2, [a-z], [A-Z])[_DECL], 1, [Define if you have the declaration of $2.]) fi undefine([gt_cv_var]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/eealloc.m40000644000175000017500000000166713004436754016031 00000000000000# eealloc.m4 serial 3 dnl Copyright (C) 2003, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_EEALLOC], [ AC_REQUIRE([gl_EEMALLOC]) AC_REQUIRE([gl_EEREALLOC]) ]) AC_DEFUN([gl_EEMALLOC], [ _AC_FUNC_MALLOC_IF( [gl_cv_func_malloc_0_nonnull=1], [gl_cv_func_malloc_0_nonnull=0]) AC_DEFINE_UNQUOTED([MALLOC_0_IS_NONNULL], [$gl_cv_func_malloc_0_nonnull], [If malloc(0) is != NULL, define this to 1. Otherwise define this to 0.]) ]) AC_DEFUN([gl_EEREALLOC], [ _AC_FUNC_REALLOC_IF( [gl_cv_func_realloc_0_nonnull=1], [gl_cv_func_realloc_0_nonnull=0]) AC_DEFINE_UNQUOTED([REALLOC_0_IS_NONNULL], [$gl_cv_func_realloc_0_nonnull], [If realloc(NULL,0) is != NULL, define this to 1. Otherwise define this to 0.]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/dup2.m40000644000175000017500000001013413004436754015264 00000000000000#serial 25 dnl Copyright (C) 2002, 2005, 2007, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_DUP2], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) m4_ifdef([gl_FUNC_DUP2_OBSOLETE], [ AC_CHECK_FUNCS_ONCE([dup2]) if test $ac_cv_func_dup2 = no; then HAVE_DUP2=0 fi ], [ AC_DEFINE([HAVE_DUP2], [1], [Define to 1 if you have the 'dup2' function.]) ]) if test $HAVE_DUP2 = 1; then AC_CACHE_CHECK([whether dup2 works], [gl_cv_func_dup2_works], [AC_RUN_IFELSE([ AC_LANG_PROGRAM( [[#include #include #include #include #include #ifndef RLIM_SAVED_CUR # define RLIM_SAVED_CUR RLIM_INFINITY #endif #ifndef RLIM_SAVED_MAX # define RLIM_SAVED_MAX RLIM_INFINITY #endif ]], [[int result = 0; int bad_fd = INT_MAX; struct rlimit rlim; if (getrlimit (RLIMIT_NOFILE, &rlim) == 0 && 0 <= rlim.rlim_cur && rlim.rlim_cur <= INT_MAX && rlim.rlim_cur != RLIM_INFINITY && rlim.rlim_cur != RLIM_SAVED_MAX && rlim.rlim_cur != RLIM_SAVED_CUR) bad_fd = rlim.rlim_cur; #ifdef FD_CLOEXEC if (fcntl (1, F_SETFD, FD_CLOEXEC) == -1) result |= 1; #endif if (dup2 (1, 1) != 1) result |= 2; #ifdef FD_CLOEXEC if (fcntl (1, F_GETFD) != FD_CLOEXEC) result |= 4; #endif close (0); if (dup2 (0, 0) != -1) result |= 8; /* Many gnulib modules require POSIX conformance of EBADF. */ if (dup2 (2, bad_fd) == -1 && errno != EBADF) result |= 16; /* Flush out some cygwin core dumps. */ if (dup2 (2, -1) != -1 || errno != EBADF) result |= 32; dup2 (2, 255); dup2 (2, 256); /* On OS/2 kLIBC, dup2() does not work on a directory fd. */ { int fd = open (".", O_RDONLY); if (fd == -1) result |= 64; else if (dup2 (fd, fd + 1) == -1) result |= 128; close (fd); } return result;]]) ], [gl_cv_func_dup2_works=yes], [gl_cv_func_dup2_works=no], [case "$host_os" in mingw*) # on this platform, dup2 always returns 0 for success gl_cv_func_dup2_works="guessing no" ;; cygwin*) # on cygwin 1.5.x, dup2(1,1) returns 0 gl_cv_func_dup2_works="guessing no" ;; aix* | freebsd*) # on AIX 7.1 and FreeBSD 6.1, dup2 (1,toobig) gives EMFILE, # not EBADF. gl_cv_func_dup2_works="guessing no" ;; haiku*) # on Haiku alpha 2, dup2(1, 1) resets FD_CLOEXEC. gl_cv_func_dup2_works="guessing no" ;; *-android*) # implemented using dup3(), which fails if oldfd == newfd gl_cv_func_dup2_works="guessing no" ;; os2*) # on OS/2 kLIBC, dup2() does not work on a directory fd. gl_cv_func_dup2_works="guessing no" ;; *) gl_cv_func_dup2_works="guessing yes" ;; esac]) ]) case "$gl_cv_func_dup2_works" in *yes) ;; *) REPLACE_DUP2=1 AC_CHECK_FUNCS([setdtablesize]) ;; esac fi dnl Replace dup2() for supporting the gnulib-defined fchdir() function, dnl to keep fchdir's bookkeeping up-to-date. m4_ifdef([gl_FUNC_FCHDIR], [ gl_TEST_FCHDIR if test $HAVE_FCHDIR = 0; then if test $HAVE_DUP2 = 1; then REPLACE_DUP2=1 fi fi ]) ]) # Prerequisites of lib/dup2.c. AC_DEFUN([gl_PREREQ_DUP2], []) gnuastro-0.2.33-8a3b/bootstrapped/m4/double-slash-root.m40000644000175000017500000000312513004436754017757 00000000000000# double-slash-root.m4 serial 4 -*- Autoconf -*- dnl Copyright (C) 2006, 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_DOUBLE_SLASH_ROOT], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_CACHE_CHECK([whether // is distinct from /], [gl_cv_double_slash_root], [ if test x"$cross_compiling" = xyes ; then # When cross-compiling, there is no way to tell whether // is special # short of a list of hosts. However, the only known hosts to date # that have a distinct // are Apollo DomainOS (too old to port to), # Cygwin, and z/OS. If anyone knows of another system for which // has # special semantics and is distinct from /, please report it to # . case $host in *-cygwin | i370-ibm-openedition) gl_cv_double_slash_root=yes ;; *) # Be optimistic and assume that / and // are the same when we # don't know. gl_cv_double_slash_root='unknown, assuming no' ;; esac else set x `ls -di / // 2>/dev/null` if test "$[2]" = "$[4]" && wc //dev/null >/dev/null 2>&1; then gl_cv_double_slash_root=no else gl_cv_double_slash_root=yes fi fi]) if test "$gl_cv_double_slash_root" = yes; then AC_DEFINE([DOUBLE_SLASH_IS_DISTINCT_ROOT], [1], [Define to 1 if // is a file system root distinct from /.]) fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/dirname.m40000644000175000017500000000105413004436754016032 00000000000000#serial 10 -*- autoconf -*- dnl Copyright (C) 2002-2006, 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_DIRNAME], [ AC_REQUIRE([gl_DIRNAME_LGPL]) ]) AC_DEFUN([gl_DIRNAME_LGPL], [ dnl Prerequisites of lib/dirname.h. AC_REQUIRE([gl_DOUBLE_SLASH_ROOT]) dnl No prerequisites of lib/basename-lgpl.c, lib/dirname-lgpl.c, dnl lib/stripslash.c. ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/ctype.m40000644000175000017500000000177513004436754015551 00000000000000# ctype_h.m4 serial 6 dnl Copyright (C) 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_CTYPE_H], [ AC_REQUIRE([gl_CTYPE_H_DEFAULTS]) dnl is always overridden, because of GNULIB_POSIXCHECK. gl_NEXT_HEADERS([ctype.h]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[#include ]], [isblank]) ]) AC_DEFUN([gl_CTYPE_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_CTYPE_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) ]) AC_DEFUN([gl_CTYPE_H_DEFAULTS], [ GNULIB_ISBLANK=0; AC_SUBST([GNULIB_ISBLANK]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_ISBLANK=1; AC_SUBST([HAVE_ISBLANK]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/configmake.m40000644000175000017500000000402113004436754016513 00000000000000# configmake.m4 serial 2 dnl Copyright (C) 2010-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # gl_CONFIGMAKE_PREP # ------------------ # Guarantee all of the standard directory variables, even when used with # autoconf 2.59 (datarootdir wasn't supported until 2.59c, and runstatedir # in 2.70) or automake 1.9.6 (pkglibexecdir wasn't supported until 1.10b, # and runstatedir in 1.14.1). AC_DEFUN([gl_CONFIGMAKE_PREP], [ dnl Technically, datadir should default to datarootdir. But if dnl autoconf is too old to provide datarootdir, then reversing the dnl definition is a reasonable compromise. Only AC_SUBST a variable dnl if it was not already defined earlier by autoconf. if test "x$datarootdir" = x; then AC_SUBST([datarootdir], ['${datadir}']) fi dnl Copy the approach used in autoconf 2.60. if test "x$docdir" = x; then AC_SUBST([docdir], [m4_ifset([AC_PACKAGE_TARNAME], ['${datarootdir}/doc/${PACKAGE_TARNAME}'], ['${datarootdir}/doc/${PACKAGE}'])]) fi dnl The remaining variables missing from autoconf 2.59 are easier. if test "x$htmldir" = x; then AC_SUBST([htmldir], ['${docdir}']) fi if test "x$dvidir" = x; then AC_SUBST([dvidir], ['${docdir}']) fi if test "x$pdfdir" = x; then AC_SUBST([pdfdir], ['${docdir}']) fi if test "x$psdir" = x; then AC_SUBST([psdir], ['${docdir}']) fi if test "x$lispdir" = x; then AC_SUBST([lispdir], ['${datarootdir}/emacs/site-lisp']) fi if test "x$localedir" = x; then AC_SUBST([localedir], ['${datarootdir}/locale']) fi dnl Added in autoconf 2.70 if test "x$runstatedir" = x; then AC_SUBST([runstatedir], ['${localstatedir}/run']) fi dnl Automake 1.9.6 only lacks pkglibexecdir; and since 1.11 merely dnl provides it without AC_SUBST, this blind use of AC_SUBST is safe. AC_SUBST([pkglibexecdir], ['${libexecdir}/${PACKAGE}']) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/codeset.m40000644000175000017500000000151213004436754016040 00000000000000# codeset.m4 serial 5 (gettext-0.18.2) dnl Copyright (C) 2000-2002, 2006, 2008-2014, 2016 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. AC_DEFUN([AM_LANGINFO_CODESET], [ AC_CACHE_CHECK([for nl_langinfo and CODESET], [am_cv_langinfo_codeset], [AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[char* cs = nl_langinfo(CODESET); return !cs;]])], [am_cv_langinfo_codeset=yes], [am_cv_langinfo_codeset=no]) ]) if test $am_cv_langinfo_codeset = yes; then AC_DEFINE([HAVE_LANGINFO_CODESET], [1], [Define if you have and nl_langinfo(CODESET).]) fi ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/close.m40000644000175000017500000000214613004436754015523 00000000000000# close.m4 serial 8 dnl Copyright (C) 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_CLOSE], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([gl_MSVC_INVAL]) if test $HAVE_MSVC_INVALID_PARAMETER_HANDLER = 1; then REPLACE_CLOSE=1 fi m4_ifdef([gl_PREREQ_SYS_H_WINSOCK2], [ gl_PREREQ_SYS_H_WINSOCK2 if test $UNISTD_H_HAVE_WINSOCK2_H = 1; then dnl Even if the 'socket' module is not used here, another part of the dnl application may use it and pass file descriptors that refer to dnl sockets to the close() function. So enable the support for sockets. REPLACE_CLOSE=1 fi ]) dnl Replace close() for supporting the gnulib-defined fchdir() function, dnl to keep fchdir's bookkeeping up-to-date. m4_ifdef([gl_FUNC_FCHDIR], [ if test $REPLACE_CLOSE = 0; then gl_TEST_FCHDIR if test $HAVE_FCHDIR = 0; then REPLACE_CLOSE=1 fi fi ]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/btowc.m40000644000175000017500000000613313004436754015534 00000000000000# btowc.m4 serial 10 dnl Copyright (C) 2008-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_BTOWC], [ AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) dnl Check whether is usable at all, first. Otherwise the test dnl program below may lead to an endless loop. See dnl . AC_REQUIRE([gl_WCHAR_H_INLINE_OK]) AC_CHECK_FUNCS_ONCE([btowc]) if test $ac_cv_func_btowc = no; then HAVE_BTOWC=0 else AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_FR]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles dnl Cygwin 1.7.2 btowc('\0') is WEOF, not 0. AC_CACHE_CHECK([whether btowc(0) is correct], [gl_cv_func_btowc_nul], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (btowc ('\0') != 0) return 1; return 0; }]])], [gl_cv_func_btowc_nul=yes], [gl_cv_func_btowc_nul=no], [ changequote(,)dnl case "$host_os" in # Guess no on Cygwin. cygwin*) gl_cv_func_btowc_nul="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_btowc_nul="guessing yes" ;; esac changequote([,])dnl ]) ]) dnl IRIX 6.5 btowc(EOF) is 0xFF, not WEOF. AC_CACHE_CHECK([whether btowc(EOF) is correct], [gl_cv_func_btowc_eof], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on IRIX. irix*) gl_cv_func_btowc_eof="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_btowc_eof="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_FR != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_FR") != NULL) { if (btowc (EOF) != WEOF) return 1; } return 0; }]])], [gl_cv_func_btowc_eof=yes], [gl_cv_func_btowc_eof=no], [:]) fi ]) case "$gl_cv_func_btowc_nul" in *yes) ;; *) REPLACE_BTOWC=1 ;; esac case "$gl_cv_func_btowc_eof" in *yes) ;; *) REPLACE_BTOWC=1 ;; esac fi ]) # Prerequisites of lib/btowc.c. AC_DEFUN([gl_PREREQ_BTOWC], [ : ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/ax_pthread.m40000644000175000017500000005052013004436765016536 00000000000000# =========================================================================== # http://www.gnu.org/software/autoconf-archive/ax_pthread.html # =========================================================================== # # SYNOPSIS # # AX_PTHREAD([ACTION-IF-FOUND[, ACTION-IF-NOT-FOUND]]) # # DESCRIPTION # # This macro figures out how to build C programs using POSIX threads. It # sets the PTHREAD_LIBS output variable to the threads library and linker # flags, and the PTHREAD_CFLAGS output variable to any special C compiler # flags that are needed. (The user can also force certain compiler # flags/libs to be tested by setting these environment variables.) # # Also sets PTHREAD_CC to any special C compiler that is needed for # multi-threaded programs (defaults to the value of CC otherwise). (This # is necessary on AIX to use the special cc_r compiler alias.) # # NOTE: You are assumed to not only compile your program with these flags, # but also to link with them as well. For example, you might link with # $PTHREAD_CC $CFLAGS $PTHREAD_CFLAGS $LDFLAGS ... $PTHREAD_LIBS $LIBS # # If you are only building threaded programs, you may wish to use these # variables in your default LIBS, CFLAGS, and CC: # # LIBS="$PTHREAD_LIBS $LIBS" # CFLAGS="$CFLAGS $PTHREAD_CFLAGS" # CC="$PTHREAD_CC" # # In addition, if the PTHREAD_CREATE_JOINABLE thread-attribute constant # has a nonstandard name, this macro defines PTHREAD_CREATE_JOINABLE to # that name (e.g. PTHREAD_CREATE_UNDETACHED on AIX). # # Also HAVE_PTHREAD_PRIO_INHERIT is defined if pthread is found and the # PTHREAD_PRIO_INHERIT symbol is defined when compiling with # PTHREAD_CFLAGS. # # ACTION-IF-FOUND is a list of shell commands to run if a threads library # is found, and ACTION-IF-NOT-FOUND is a list of commands to run it if it # is not found. If ACTION-IF-FOUND is not specified, the default action # will define HAVE_PTHREAD. # # Please let the authors know if this macro fails on any platform, or if # you have any other suggestions or comments. This macro was based on work # by SGJ on autoconf scripts for FFTW (http://www.fftw.org/) (with help # from M. Frigo), as well as ac_pthread and hb_pthread macros posted by # Alejandro Forero Cuervo to the autoconf macro repository. We are also # grateful for the helpful feedback of numerous users. # # Updated for Autoconf 2.68 by Daniel Richard G. # # LICENSE # # Copyright (c) 2008 Steven G. Johnson # Copyright (c) 2011 Daniel Richard G. # # This program is free software: you can redistribute it and/or modify it # under the terms of the GNU General Public License as published by the # Free Software Foundation, either version 3 of the License, or (at your # option) any later version. # # This program is distributed in the hope that it will be useful, but # WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General # Public License for more details. # # You should have received a copy of the GNU General Public License along # with this program. If not, see . # # As a special exception, the respective Autoconf Macro's copyright owner # gives unlimited permission to copy, distribute and modify the configure # scripts that are the output of Autoconf when processing the Macro. You # need not follow the terms of the GNU General Public License when using # or distributing such scripts, even though portions of the text of the # Macro appear in them. The GNU General Public License (GPL) does govern # all other use of the material that constitutes the Autoconf Macro. # # This special exception to the GPL applies to versions of the Autoconf # Macro released by the Autoconf Archive. When you make and distribute a # modified version of the Autoconf Macro, you may extend this special # exception to the GPL to apply to your modified version as well. #serial 23 AU_ALIAS([ACX_PTHREAD], [AX_PTHREAD]) AC_DEFUN([AX_PTHREAD], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_PROG_SED]) AC_LANG_PUSH([C]) ax_pthread_ok=no # We used to check for pthread.h first, but this fails if pthread.h # requires special compiler flags (e.g. on Tru64 or Sequent). # It gets checked for in the link test anyway. # First of all, check if the user has set any of the PTHREAD_LIBS, # etcetera environment variables, and if threads linking works using # them: if test "x$PTHREAD_CFLAGS$PTHREAD_LIBS" != "x"; then ax_pthread_save_CC="$CC" ax_pthread_save_CFLAGS="$CFLAGS" ax_pthread_save_LIBS="$LIBS" AS_IF([test "x$PTHREAD_CC" != "x"], [CC="$PTHREAD_CC"]) CFLAGS="$CFLAGS $PTHREAD_CFLAGS" LIBS="$PTHREAD_LIBS $LIBS" AC_MSG_CHECKING([for pthread_join using $CC $PTHREAD_CFLAGS $PTHREAD_LIBS]) AC_LINK_IFELSE([AC_LANG_CALL([], [pthread_join])], [ax_pthread_ok=yes]) AC_MSG_RESULT([$ax_pthread_ok]) if test "x$ax_pthread_ok" = "xno"; then PTHREAD_LIBS="" PTHREAD_CFLAGS="" fi CC="$ax_pthread_save_CC" CFLAGS="$ax_pthread_save_CFLAGS" LIBS="$ax_pthread_save_LIBS" fi # We must check for the threads library under a number of different # names; the ordering is very important because some systems # (e.g. DEC) have both -lpthread and -lpthreads, where one of the # libraries is broken (non-POSIX). # Create a list of thread flags to try. Items starting with a "-" are # C compiler flags, and other items are library names, except for "none" # which indicates that we try without any flags at all, and "pthread-config" # which is a program returning the flags for the Pth emulation library. ax_pthread_flags="pthreads none -Kthread -pthread -pthreads -mthreads pthread --thread-safe -mt pthread-config" # The ordering *is* (sometimes) important. Some notes on the # individual items follow: # pthreads: AIX (must check this before -lpthread) # none: in case threads are in libc; should be tried before -Kthread and # other compiler flags to prevent continual compiler warnings # -Kthread: Sequent (threads in libc, but -Kthread needed for pthread.h) # -pthread: Linux/gcc (kernel threads), BSD/gcc (userland threads), Tru64 # (Note: HP C rejects this with "bad form for `-t' option") # -pthreads: Solaris/gcc (Note: HP C also rejects) # -mt: Sun Workshop C (may only link SunOS threads [-lthread], but it # doesn't hurt to check since this sometimes defines pthreads and # -D_REENTRANT too), HP C (must be checked before -lpthread, which # is present but should not be used directly; and before -mthreads, # because the compiler interprets this as "-mt" + "-hreads") # -mthreads: Mingw32/gcc, Lynx/gcc # pthread: Linux, etcetera # --thread-safe: KAI C++ # pthread-config: use pthread-config program (for GNU Pth library) case $host_os in freebsd*) # -kthread: FreeBSD kernel threads (preferred to -pthread since SMP-able) # lthread: LinuxThreads port on FreeBSD (also preferred to -pthread) ax_pthread_flags="-kthread lthread $ax_pthread_flags" ;; hpux*) # From the cc(1) man page: "[-mt] Sets various -D flags to enable # multi-threading and also sets -lpthread." ax_pthread_flags="-mt -pthread pthread $ax_pthread_flags" ;; openedition*) # IBM z/OS requires a feature-test macro to be defined in order to # enable POSIX threads at all, so give the user a hint if this is # not set. (We don't define these ourselves, as they can affect # other portions of the system API in unpredictable ways.) AC_EGREP_CPP([AX_PTHREAD_ZOS_MISSING], [ # if !defined(_OPEN_THREADS) && !defined(_UNIX03_THREADS) AX_PTHREAD_ZOS_MISSING # endif ], [AC_MSG_WARN([IBM z/OS requires -D_OPEN_THREADS or -D_UNIX03_THREADS to enable pthreads support.])]) ;; solaris*) # On Solaris (at least, for some versions), libc contains stubbed # (non-functional) versions of the pthreads routines, so link-based # tests will erroneously succeed. (N.B.: The stubs are missing # pthread_cleanup_push, or rather a function called by this macro, # so we could check for that, but who knows whether they'll stub # that too in a future libc.) So we'll check first for the # standard Solaris way of linking pthreads (-mt -lpthread). ax_pthread_flags="-mt,pthread pthread $ax_pthread_flags" ;; esac # GCC generally uses -pthread, or -pthreads on some platforms (e.g. SPARC) AS_IF([test "x$GCC" = "xyes"], [ax_pthread_flags="-pthread -pthreads $ax_pthread_flags"]) # The presence of a feature test macro requesting re-entrant function # definitions is, on some systems, a strong hint that pthreads support is # correctly enabled case $host_os in darwin* | hpux* | linux* | osf* | solaris*) ax_pthread_check_macro="_REENTRANT" ;; aix*) ax_pthread_check_macro="_THREAD_SAFE" ;; *) ax_pthread_check_macro="--" ;; esac AS_IF([test "x$ax_pthread_check_macro" = "x--"], [ax_pthread_check_cond=0], [ax_pthread_check_cond="!defined($ax_pthread_check_macro)"]) # Are we compiling with Clang? AC_CACHE_CHECK([whether $CC is Clang], [ax_cv_PTHREAD_CLANG], [ax_cv_PTHREAD_CLANG=no # Note that Autoconf sets GCC=yes for Clang as well as GCC if test "x$GCC" = "xyes"; then AC_EGREP_CPP([AX_PTHREAD_CC_IS_CLANG], [/* Note: Clang 2.7 lacks __clang_[a-z]+__ */ # if defined(__clang__) && defined(__llvm__) AX_PTHREAD_CC_IS_CLANG # endif ], [ax_cv_PTHREAD_CLANG=yes]) fi ]) ax_pthread_clang="$ax_cv_PTHREAD_CLANG" ax_pthread_clang_warning=no # Clang needs special handling, because older versions handle the -pthread # option in a rather... idiosyncratic way if test "x$ax_pthread_clang" = "xyes"; then # Clang takes -pthread; it has never supported any other flag # (Note 1: This will need to be revisited if a system that Clang # supports has POSIX threads in a separate library. This tends not # to be the way of modern systems, but it's conceivable.) # (Note 2: On some systems, notably Darwin, -pthread is not needed # to get POSIX threads support; the API is always present and # active. We could reasonably leave PTHREAD_CFLAGS empty. But # -pthread does define _REENTRANT, and while the Darwin headers # ignore this macro, third-party headers might not.) PTHREAD_CFLAGS="-pthread" PTHREAD_LIBS= ax_pthread_ok=yes # However, older versions of Clang make a point of warning the user # that, in an invocation where only linking and no compilation is # taking place, the -pthread option has no effect ("argument unused # during compilation"). They expect -pthread to be passed in only # when source code is being compiled. # # Problem is, this is at odds with the way Automake and most other # C build frameworks function, which is that the same flags used in # compilation (CFLAGS) are also used in linking. Many systems # supported by AX_PTHREAD require exactly this for POSIX threads # support, and in fact it is often not straightforward to specify a # flag that is used only in the compilation phase and not in # linking. Such a scenario is extremely rare in practice. # # Even though use of the -pthread flag in linking would only print # a warning, this can be a nuisance for well-run software projects # that build with -Werror. So if the active version of Clang has # this misfeature, we search for an option to squash it. AC_CACHE_CHECK([whether Clang needs flag to prevent "argument unused" warning when linking with -pthread], [ax_cv_PTHREAD_CLANG_NO_WARN_FLAG], [ax_cv_PTHREAD_CLANG_NO_WARN_FLAG=unknown # Create an alternate version of $ac_link that compiles and # links in two steps (.c -> .o, .o -> exe) instead of one # (.c -> exe), because the warning occurs only in the second # step ax_pthread_save_ac_link="$ac_link" ax_pthread_sed='s/conftest\.\$ac_ext/conftest.$ac_objext/g' ax_pthread_link_step=`$as_echo "$ac_link" | sed "$ax_pthread_sed"` ax_pthread_2step_ac_link="($ac_compile) && (echo ==== >&5) && ($ax_pthread_link_step)" ax_pthread_save_CFLAGS="$CFLAGS" for ax_pthread_try in '' -Qunused-arguments -Wno-unused-command-line-argument unknown; do AS_IF([test "x$ax_pthread_try" = "xunknown"], [break]) CFLAGS="-Werror -Wunknown-warning-option $ax_pthread_try -pthread $ax_pthread_save_CFLAGS" ac_link="$ax_pthread_save_ac_link" AC_LINK_IFELSE([AC_LANG_SOURCE([[int main(void){return 0;}]])], [ac_link="$ax_pthread_2step_ac_link" AC_LINK_IFELSE([AC_LANG_SOURCE([[int main(void){return 0;}]])], [break]) ]) done ac_link="$ax_pthread_save_ac_link" CFLAGS="$ax_pthread_save_CFLAGS" AS_IF([test "x$ax_pthread_try" = "x"], [ax_pthread_try=no]) ax_cv_PTHREAD_CLANG_NO_WARN_FLAG="$ax_pthread_try" ]) case "$ax_cv_PTHREAD_CLANG_NO_WARN_FLAG" in no | unknown) ;; *) PTHREAD_CFLAGS="$ax_cv_PTHREAD_CLANG_NO_WARN_FLAG $PTHREAD_CFLAGS" ;; esac fi # $ax_pthread_clang = yes if test "x$ax_pthread_ok" = "xno"; then for ax_pthread_try_flag in $ax_pthread_flags; do case $ax_pthread_try_flag in none) AC_MSG_CHECKING([whether pthreads work without any flags]) ;; -mt,pthread) AC_MSG_CHECKING([whether pthreads work with -mt -lpthread]) PTHREAD_CFLAGS="-mt" PTHREAD_LIBS="-lpthread" ;; -*) AC_MSG_CHECKING([whether pthreads work with $ax_pthread_try_flag]) PTHREAD_CFLAGS="$ax_pthread_try_flag" ;; pthread-config) AC_CHECK_PROG([ax_pthread_config], [pthread-config], [yes], [no]) AS_IF([test "x$ax_pthread_config" = "xno"], [continue]) PTHREAD_CFLAGS="`pthread-config --cflags`" PTHREAD_LIBS="`pthread-config --ldflags` `pthread-config --libs`" ;; *) AC_MSG_CHECKING([for the pthreads library -l$ax_pthread_try_flag]) PTHREAD_LIBS="-l$ax_pthread_try_flag" ;; esac ax_pthread_save_CFLAGS="$CFLAGS" ax_pthread_save_LIBS="$LIBS" CFLAGS="$CFLAGS $PTHREAD_CFLAGS" LIBS="$PTHREAD_LIBS $LIBS" # Check for various functions. We must include pthread.h, # since some functions may be macros. (On the Sequent, we # need a special flag -Kthread to make this header compile.) # We check for pthread_join because it is in -lpthread on IRIX # while pthread_create is in libc. We check for pthread_attr_init # due to DEC craziness with -lpthreads. We check for # pthread_cleanup_push because it is one of the few pthread # functions on Solaris that doesn't have a non-functional libc stub. # We try pthread_create on general principles. AC_LINK_IFELSE([AC_LANG_PROGRAM([#include # if $ax_pthread_check_cond # error "$ax_pthread_check_macro must be defined" # endif static void routine(void *a) { a = 0; } static void *start_routine(void *a) { return a; }], [pthread_t th; pthread_attr_t attr; pthread_create(&th, 0, start_routine, 0); pthread_join(th, 0); pthread_attr_init(&attr); pthread_cleanup_push(routine, 0); pthread_cleanup_pop(0) /* ; */])], [ax_pthread_ok=yes], []) CFLAGS="$ax_pthread_save_CFLAGS" LIBS="$ax_pthread_save_LIBS" AC_MSG_RESULT([$ax_pthread_ok]) AS_IF([test "x$ax_pthread_ok" = "xyes"], [break]) PTHREAD_LIBS="" PTHREAD_CFLAGS="" done fi # Various other checks: if test "x$ax_pthread_ok" = "xyes"; then ax_pthread_save_CFLAGS="$CFLAGS" ax_pthread_save_LIBS="$LIBS" CFLAGS="$CFLAGS $PTHREAD_CFLAGS" LIBS="$PTHREAD_LIBS $LIBS" # Detect AIX lossage: JOINABLE attribute is called UNDETACHED. AC_CACHE_CHECK([for joinable pthread attribute], [ax_cv_PTHREAD_JOINABLE_ATTR], [ax_cv_PTHREAD_JOINABLE_ATTR=unknown for ax_pthread_attr in PTHREAD_CREATE_JOINABLE PTHREAD_CREATE_UNDETACHED; do AC_LINK_IFELSE([AC_LANG_PROGRAM([#include ], [int attr = $ax_pthread_attr; return attr /* ; */])], [ax_cv_PTHREAD_JOINABLE_ATTR=$ax_pthread_attr; break], []) done ]) AS_IF([test "x$ax_cv_PTHREAD_JOINABLE_ATTR" != "xunknown" && \ test "x$ax_cv_PTHREAD_JOINABLE_ATTR" != "xPTHREAD_CREATE_JOINABLE" && \ test "x$ax_pthread_joinable_attr_defined" != "xyes"], [AC_DEFINE_UNQUOTED([PTHREAD_CREATE_JOINABLE], [$ax_cv_PTHREAD_JOINABLE_ATTR], [Define to necessary symbol if this constant uses a non-standard name on your system.]) ax_pthread_joinable_attr_defined=yes ]) AC_CACHE_CHECK([whether more special flags are required for pthreads], [ax_cv_PTHREAD_SPECIAL_FLAGS], [ax_cv_PTHREAD_SPECIAL_FLAGS=no case $host_os in solaris*) ax_cv_PTHREAD_SPECIAL_FLAGS="-D_POSIX_PTHREAD_SEMANTICS" ;; esac ]) AS_IF([test "x$ax_cv_PTHREAD_SPECIAL_FLAGS" != "xno" && \ test "x$ax_pthread_special_flags_added" != "xyes"], [PTHREAD_CFLAGS="$ax_cv_PTHREAD_SPECIAL_FLAGS $PTHREAD_CFLAGS" ax_pthread_special_flags_added=yes]) AC_CACHE_CHECK([for PTHREAD_PRIO_INHERIT], [ax_cv_PTHREAD_PRIO_INHERIT], [AC_LINK_IFELSE([AC_LANG_PROGRAM([[#include ]], [[int i = PTHREAD_PRIO_INHERIT;]])], [ax_cv_PTHREAD_PRIO_INHERIT=yes], [ax_cv_PTHREAD_PRIO_INHERIT=no]) ]) AS_IF([test "x$ax_cv_PTHREAD_PRIO_INHERIT" = "xyes" && \ test "x$ax_pthread_prio_inherit_defined" != "xyes"], [AC_DEFINE([HAVE_PTHREAD_PRIO_INHERIT], [1], [Have PTHREAD_PRIO_INHERIT.]) ax_pthread_prio_inherit_defined=yes ]) CFLAGS="$ax_pthread_save_CFLAGS" LIBS="$ax_pthread_save_LIBS" # More AIX lossage: compile with *_r variant if test "x$GCC" != "xyes"; then case $host_os in aix*) AS_CASE(["x/$CC"], [x*/c89|x*/c89_128|x*/c99|x*/c99_128|x*/cc|x*/cc128|x*/xlc|x*/xlc_v6|x*/xlc128|x*/xlc128_v6], [#handle absolute path differently from PATH based program lookup AS_CASE(["x$CC"], [x/*], [AS_IF([AS_EXECUTABLE_P([${CC}_r])],[PTHREAD_CC="${CC}_r"])], [AC_CHECK_PROGS([PTHREAD_CC],[${CC}_r],[$CC])])]) ;; esac fi fi test -n "$PTHREAD_CC" || PTHREAD_CC="$CC" AC_SUBST([PTHREAD_LIBS]) AC_SUBST([PTHREAD_CFLAGS]) AC_SUBST([PTHREAD_CC]) # Finally, execute ACTION-IF-FOUND/ACTION-IF-NOT-FOUND: if test "x$ax_pthread_ok" = "xyes"; then ifelse([$1],,[AC_DEFINE([HAVE_PTHREAD],[1],[Define if you have POSIX threads libraries and header files.])],[$1]) : else ax_pthread_ok=no $2 fi AC_LANG_POP ])dnl AX_PTHREAD gnuastro-0.2.33-8a3b/bootstrapped/m4/ax_compare_version.m40000644000175000017500000001465213004436765020310 00000000000000# =========================================================================== # http://www.gnu.org/software/autoconf-archive/ax_compare_version.html # =========================================================================== # # SYNOPSIS # # AX_COMPARE_VERSION(VERSION_A, OP, VERSION_B, [ACTION-IF-TRUE], [ACTION-IF-FALSE]) # # DESCRIPTION # # This macro compares two version strings. Due to the various number of # minor-version numbers that can exist, and the fact that string # comparisons are not compatible with numeric comparisons, this is not # necessarily trivial to do in a autoconf script. This macro makes doing # these comparisons easy. # # The six basic comparisons are available, as well as checking equality # limited to a certain number of minor-version levels. # # The operator OP determines what type of comparison to do, and can be one # of: # # eq - equal (test A == B) # ne - not equal (test A != B) # le - less than or equal (test A <= B) # ge - greater than or equal (test A >= B) # lt - less than (test A < B) # gt - greater than (test A > B) # # Additionally, the eq and ne operator can have a number after it to limit # the test to that number of minor versions. # # eq0 - equal up to the length of the shorter version # ne0 - not equal up to the length of the shorter version # eqN - equal up to N sub-version levels # neN - not equal up to N sub-version levels # # When the condition is true, shell commands ACTION-IF-TRUE are run, # otherwise shell commands ACTION-IF-FALSE are run. The environment # variable 'ax_compare_version' is always set to either 'true' or 'false' # as well. # # Examples: # # AX_COMPARE_VERSION([3.15.7],[lt],[3.15.8]) # AX_COMPARE_VERSION([3.15],[lt],[3.15.8]) # # would both be true. # # AX_COMPARE_VERSION([3.15.7],[eq],[3.15.8]) # AX_COMPARE_VERSION([3.15],[gt],[3.15.8]) # # would both be false. # # AX_COMPARE_VERSION([3.15.7],[eq2],[3.15.8]) # # would be true because it is only comparing two minor versions. # # AX_COMPARE_VERSION([3.15.7],[eq0],[3.15]) # # would be true because it is only comparing the lesser number of minor # versions of the two values. # # Note: The characters that separate the version numbers do not matter. An # empty string is the same as version 0. OP is evaluated by autoconf, not # configure, so must be a string, not a variable. # # The author would like to acknowledge Guido Draheim whose advice about # the m4_case and m4_ifvaln functions make this macro only include the # portions necessary to perform the specific comparison specified by the # OP argument in the final configure script. # # LICENSE # # Copyright (c) 2008 Tim Toolan # # Copying and distribution of this file, with or without modification, are # permitted in any medium without royalty provided the copyright notice # and this notice are preserved. This file is offered as-is, without any # warranty. #serial 11 dnl ######################################################################### AC_DEFUN([AX_COMPARE_VERSION], [ AC_REQUIRE([AC_PROG_AWK]) # Used to indicate true or false condition ax_compare_version=false # Convert the two version strings to be compared into a format that # allows a simple string comparison. The end result is that a version # string of the form 1.12.5-r617 will be converted to the form # 0001001200050617. In other words, each number is zero padded to four # digits, and non digits are removed. AS_VAR_PUSHDEF([A],[ax_compare_version_A]) A=`echo "$1" | sed -e 's/\([[0-9]]*\)/Z\1Z/g' \ -e 's/Z\([[0-9]]\)Z/Z0\1Z/g' \ -e 's/Z\([[0-9]][[0-9]]\)Z/Z0\1Z/g' \ -e 's/Z\([[0-9]][[0-9]][[0-9]]\)Z/Z0\1Z/g' \ -e 's/[[^0-9]]//g'` AS_VAR_PUSHDEF([B],[ax_compare_version_B]) B=`echo "$3" | sed -e 's/\([[0-9]]*\)/Z\1Z/g' \ -e 's/Z\([[0-9]]\)Z/Z0\1Z/g' \ -e 's/Z\([[0-9]][[0-9]]\)Z/Z0\1Z/g' \ -e 's/Z\([[0-9]][[0-9]][[0-9]]\)Z/Z0\1Z/g' \ -e 's/[[^0-9]]//g'` dnl # In the case of le, ge, lt, and gt, the strings are sorted as necessary dnl # then the first line is used to determine if the condition is true. dnl # The sed right after the echo is to remove any indented white space. m4_case(m4_tolower($2), [lt],[ ax_compare_version=`echo "x$A x$B" | sed 's/^ *//' | sort -r | sed "s/x${A}/false/;s/x${B}/true/;1q"` ], [gt],[ ax_compare_version=`echo "x$A x$B" | sed 's/^ *//' | sort | sed "s/x${A}/false/;s/x${B}/true/;1q"` ], [le],[ ax_compare_version=`echo "x$A x$B" | sed 's/^ *//' | sort | sed "s/x${A}/true/;s/x${B}/false/;1q"` ], [ge],[ ax_compare_version=`echo "x$A x$B" | sed 's/^ *//' | sort -r | sed "s/x${A}/true/;s/x${B}/false/;1q"` ],[ dnl Split the operator from the subversion count if present. m4_bmatch(m4_substr($2,2), [0],[ # A count of zero means use the length of the shorter version. # Determine the number of characters in A and B. ax_compare_version_len_A=`echo "$A" | $AWK '{print(length)}'` ax_compare_version_len_B=`echo "$B" | $AWK '{print(length)}'` # Set A to no more than B's length and B to no more than A's length. A=`echo "$A" | sed "s/\(.\{$ax_compare_version_len_B\}\).*/\1/"` B=`echo "$B" | sed "s/\(.\{$ax_compare_version_len_A\}\).*/\1/"` ], [[0-9]+],[ # A count greater than zero means use only that many subversions A=`echo "$A" | sed "s/\(\([[0-9]]\{4\}\)\{m4_substr($2,2)\}\).*/\1/"` B=`echo "$B" | sed "s/\(\([[0-9]]\{4\}\)\{m4_substr($2,2)\}\).*/\1/"` ], [.+],[ AC_WARNING( [illegal OP numeric parameter: $2]) ],[]) # Pad zeros at end of numbers to make same length. ax_compare_version_tmp_A="$A`echo $B | sed 's/./0/g'`" B="$B`echo $A | sed 's/./0/g'`" A="$ax_compare_version_tmp_A" # Check for equality or inequality as necessary. m4_case(m4_tolower(m4_substr($2,0,2)), [eq],[ test "x$A" = "x$B" && ax_compare_version=true ], [ne],[ test "x$A" != "x$B" && ax_compare_version=true ],[ AC_WARNING([illegal OP parameter: $2]) ]) ]) AS_VAR_POPDEF([A])dnl AS_VAR_POPDEF([B])dnl dnl # Execute ACTION-IF-TRUE / ACTION-IF-FALSE. if test "$ax_compare_version" = "true" ; then m4_ifvaln([$4],[$4],[:])dnl m4_ifvaln([$5],[else $5])dnl fi ]) dnl AX_COMPARE_VERSION gnuastro-0.2.33-8a3b/bootstrapped/m4/argp.m40000644000175000017500000000542613004436754015353 00000000000000# argp.m4 serial 15 dnl Copyright (C) 2003-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_ARGP], [ AC_REQUIRE([AC_C_INLINE]) AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) AC_CHECK_DECLS([program_invocation_name], [], [AC_DEFINE([GNULIB_PROGRAM_INVOCATION_NAME], [1], [Define to 1 to add extern declaration of program_invocation_name to argp.h])], [[#include ]]) AC_CHECK_DECLS([program_invocation_short_name], [], [AC_DEFINE([GNULIB_PROGRAM_INVOCATION_SHORT_NAME], [1], [Define to 1 to add extern declaration of program_invocation_short_name to argp.h])], [[#include ]]) # Check if program_invocation_name and program_invocation_short_name # are defined elsewhere. It is improbable that only one of them will # be defined and other not, I prefer to stay on the safe side and to # test each one separately. AC_MSG_CHECKING([whether program_invocation_name is defined]) AC_LINK_IFELSE([AC_LANG_PROGRAM([[#include ]], [[program_invocation_name = "test";]])], [AC_DEFINE([HAVE_PROGRAM_INVOCATION_NAME], [1], [Define if program_invocation_name is defined]) AC_MSG_RESULT([yes])], [AC_MSG_RESULT([no])]) AC_MSG_CHECKING([whether program_invocation_short_name is defined]) AC_LINK_IFELSE([AC_LANG_PROGRAM([[#include ]], [[program_invocation_short_name = "test";]])], [AC_DEFINE([HAVE_PROGRAM_INVOCATION_SHORT_NAME], [1], [Define if program_invocation_short_name is defined]) AC_MSG_RESULT([yes])], [AC_MSG_RESULT([no])]) AC_CHECK_DECLS_ONCE([clearerr_unlocked]) AC_CHECK_DECLS_ONCE([feof_unlocked]) AC_CHECK_DECLS_ONCE([ferror_unlocked]) AC_CHECK_DECLS_ONCE([fflush_unlocked]) AC_CHECK_DECLS_ONCE([fgets_unlocked]) AC_CHECK_DECLS_ONCE([fputc_unlocked]) AC_CHECK_DECLS_ONCE([fputs_unlocked]) AC_CHECK_DECLS_ONCE([fread_unlocked]) AC_CHECK_DECLS_ONCE([fwrite_unlocked]) AC_CHECK_DECLS_ONCE([getc_unlocked]) AC_CHECK_DECLS_ONCE([getchar_unlocked]) AC_CHECK_DECLS_ONCE([putc_unlocked]) AC_CHECK_DECLS_ONCE([putchar_unlocked]) AC_CHECK_FUNCS_ONCE([flockfile funlockfile]) AC_CHECK_HEADERS_ONCE([features.h linewrap.h]) AC_REQUIRE([AC_FUNC_STRERROR_R]) ]) dnl argp-parse.c depends on GNU getopt internals, therefore use GNU getopt dnl always. AC_DEFUN([gl_REPLACE_GETOPT_ALWAYS], []) gnuastro-0.2.33-8a3b/bootstrapped/m4/alloca.m40000644000175000017500000001037213004436754015651 00000000000000# alloca.m4 serial 14 dnl Copyright (C) 2002-2004, 2006-2007, 2009-2016 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_ALLOCA], [ AC_REQUIRE([AC_FUNC_ALLOCA]) if test $ac_cv_func_alloca_works = no; then gl_PREREQ_ALLOCA fi # Define an additional variable used in the Makefile substitution. if test $ac_cv_working_alloca_h = yes; then AC_CACHE_CHECK([for alloca as a compiler built-in], [gl_cv_rpl_alloca], [ AC_EGREP_CPP([Need own alloca], [ #if defined __GNUC__ || defined _AIX || defined _MSC_VER Need own alloca #endif ], [gl_cv_rpl_alloca=yes], [gl_cv_rpl_alloca=no]) ]) if test $gl_cv_rpl_alloca = yes; then dnl OK, alloca can be implemented through a compiler built-in. AC_DEFINE([HAVE_ALLOCA], [1], [Define to 1 if you have 'alloca' after including , a header that may be supplied by this distribution.]) ALLOCA_H=alloca.h else dnl alloca exists as a library function, i.e. it is slow and probably dnl a memory leak. Don't define HAVE_ALLOCA in this case. ALLOCA_H= fi else ALLOCA_H=alloca.h fi AC_SUBST([ALLOCA_H]) AM_CONDITIONAL([GL_GENERATE_ALLOCA_H], [test -n "$ALLOCA_H"]) ]) # Prerequisites of lib/alloca.c. # STACK_DIRECTION is already handled by AC_FUNC_ALLOCA. AC_DEFUN([gl_PREREQ_ALLOCA], [:]) # This works around a bug in autoconf <= 2.68. # See . m4_version_prereq([2.69], [] ,[ # This is taken from the following Autoconf patch: # http://git.savannah.gnu.org/cgit/autoconf.git/commit/?id=6cd9f12520b0d6f76d3230d7565feba1ecf29497 # _AC_LIBOBJ_ALLOCA # ----------------- # Set up the LIBOBJ replacement of 'alloca'. Well, not exactly # AC_LIBOBJ since we actually set the output variable 'ALLOCA'. # Nevertheless, for Automake, AC_LIBSOURCES it. m4_define([_AC_LIBOBJ_ALLOCA], [# The SVR3 libPW and SVR4 libucb both contain incompatible functions # that cause trouble. Some versions do not even contain alloca or # contain a buggy version. If you still want to use their alloca, # use ar to extract alloca.o from them instead of compiling alloca.c. AC_LIBSOURCES(alloca.c) AC_SUBST([ALLOCA], [\${LIBOBJDIR}alloca.$ac_objext])dnl AC_DEFINE(C_ALLOCA, 1, [Define to 1 if using 'alloca.c'.]) AC_CACHE_CHECK(whether 'alloca.c' needs Cray hooks, ac_cv_os_cray, [AC_EGREP_CPP(webecray, [#if defined CRAY && ! defined CRAY2 webecray #else wenotbecray #endif ], ac_cv_os_cray=yes, ac_cv_os_cray=no)]) if test $ac_cv_os_cray = yes; then for ac_func in _getb67 GETB67 getb67; do AC_CHECK_FUNC($ac_func, [AC_DEFINE_UNQUOTED(CRAY_STACKSEG_END, $ac_func, [Define to one of '_getb67', 'GETB67', 'getb67' for Cray-2 and Cray-YMP systems. This function is required for 'alloca.c' support on those systems.]) break]) done fi AC_CACHE_CHECK([stack direction for C alloca], [ac_cv_c_stack_direction], [AC_RUN_IFELSE([AC_LANG_SOURCE( [AC_INCLUDES_DEFAULT int find_stack_direction (int *addr, int depth) { int dir, dummy = 0; if (! addr) addr = &dummy; *addr = addr < &dummy ? 1 : addr == &dummy ? 0 : -1; dir = depth ? find_stack_direction (addr, depth - 1) : 0; return dir + dummy; } int main (int argc, char **argv) { return find_stack_direction (0, argc + !argv + 20) < 0; }])], [ac_cv_c_stack_direction=1], [ac_cv_c_stack_direction=-1], [ac_cv_c_stack_direction=0])]) AH_VERBATIM([STACK_DIRECTION], [/* If using the C implementation of alloca, define if you know the direction of stack growth for your system; otherwise it will be automatically deduced at runtime. STACK_DIRECTION > 0 => grows toward higher addresses STACK_DIRECTION < 0 => grows toward lower addresses STACK_DIRECTION = 0 => direction of growth unknown */ @%:@undef STACK_DIRECTION])dnl AC_DEFINE_UNQUOTED(STACK_DIRECTION, $ac_cv_c_stack_direction) ])# _AC_LIBOBJ_ALLOCA ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/absolute-header.m40000644000175000017500000001034713004436754017464 00000000000000# absolute-header.m4 serial 16 dnl Copyright (C) 2006-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Derek Price. # gl_ABSOLUTE_HEADER(HEADER1 HEADER2 ...) # --------------------------------------- # Find the absolute name of a header file, testing first if the header exists. # If the header were sys/inttypes.h, this macro would define # ABSOLUTE_SYS_INTTYPES_H to the '""' quoted absolute name of sys/inttypes.h # in config.h # (e.g. '#define ABSOLUTE_SYS_INTTYPES_H "///usr/include/sys/inttypes.h"'). # The three "///" are to pacify Sun C 5.8, which otherwise would say # "warning: #include of /usr/include/... may be non-portable". # Use '""', not '<>', so that the /// cannot be confused with a C99 comment. # Note: This macro assumes that the header file is not empty after # preprocessing, i.e. it does not only define preprocessor macros but also # provides some type/enum definitions or function/variable declarations. AC_DEFUN([gl_ABSOLUTE_HEADER], [AC_REQUIRE([AC_CANONICAL_HOST]) AC_LANG_PREPROC_REQUIRE()dnl dnl FIXME: gl_absolute_header and ac_header_exists must be used unquoted dnl until we can assume autoconf 2.64 or newer. m4_foreach_w([gl_HEADER_NAME], [$1], [AS_VAR_PUSHDEF([gl_absolute_header], [gl_cv_absolute_]m4_defn([gl_HEADER_NAME]))dnl AC_CACHE_CHECK([absolute name of <]m4_defn([gl_HEADER_NAME])[>], m4_defn([gl_absolute_header]), [AS_VAR_PUSHDEF([ac_header_exists], [ac_cv_header_]m4_defn([gl_HEADER_NAME]))dnl AC_CHECK_HEADERS_ONCE(m4_defn([gl_HEADER_NAME]))dnl if test AS_VAR_GET(ac_header_exists) = yes; then gl_ABSOLUTE_HEADER_ONE(m4_defn([gl_HEADER_NAME])) fi AS_VAR_POPDEF([ac_header_exists])dnl ])dnl AC_DEFINE_UNQUOTED(AS_TR_CPP([ABSOLUTE_]m4_defn([gl_HEADER_NAME])), ["AS_VAR_GET(gl_absolute_header)"], [Define this to an absolute name of <]m4_defn([gl_HEADER_NAME])[>.]) AS_VAR_POPDEF([gl_absolute_header])dnl ])dnl ])# gl_ABSOLUTE_HEADER # gl_ABSOLUTE_HEADER_ONE(HEADER) # ------------------------------ # Like gl_ABSOLUTE_HEADER, except that: # - it assumes that the header exists, # - it uses the current CPPFLAGS, # - it does not cache the result, # - it is silent. AC_DEFUN([gl_ABSOLUTE_HEADER_ONE], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_LANG_CONFTEST([AC_LANG_SOURCE([[#include <]]m4_dquote([$1])[[>]])]) dnl AIX "xlc -E" and "cc -E" omit #line directives for header files dnl that contain only a #include of other header files and no dnl non-comment tokens of their own. This leads to a failure to dnl detect the absolute name of , , dnl and others. The workaround is to force preservation of comments dnl through option -C. This ensures all necessary #line directives dnl are present. GCC supports option -C as well. case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac changequote(,) case "$host_os" in mingw*) dnl For the sake of native Windows compilers (excluding gcc), dnl treat backslash as a directory separator, like /. dnl Actually, these compilers use a double-backslash as dnl directory separator, inside the dnl # line "filename" dnl directives. gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac dnl A sed expression that turns a string into a basic regular dnl expression, for use within "/.../". gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo '$1' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' changequote([,]) dnl eval is necessary to expand gl_absname_cpp. dnl Ultrix and Pyramid sh refuse to redirect output of eval, dnl so use subshell. AS_VAR_SET([gl_cv_absolute_]AS_TR_SH([[$1]]), [`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&AS_MESSAGE_LOG_FD | sed -n "$gl_absolute_header_sed"`]) ]) gnuastro-0.2.33-8a3b/bootstrapped/m4/00gnulib.m40000644000175000017500000000415213004436754016035 00000000000000# 00gnulib.m4 serial 3 dnl Copyright (C) 2009-2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl This file must be named something that sorts before all other dnl gnulib-provided .m4 files. It is needed until such time as we can dnl assume Autoconf 2.64, with its improved AC_DEFUN_ONCE and dnl m4_divert semantics. # Until autoconf 2.63, handling of the diversion stack required m4_init # to be called first; but this does not happen with aclocal. Wrapping # the entire execution in another layer of the diversion stack fixes this. # Worse, prior to autoconf 2.62, m4_wrap depended on the underlying m4 # for whether it was FIFO or LIFO; in order to properly balance with # m4_init, we need to undo our push just before anything wrapped within # the m4_init body. The way to ensure this is to wrap both sides of # m4_init with a one-shot macro that does the pop at the right time. m4_ifndef([_m4_divert_diversion], [m4_divert_push([KILL]) m4_define([gl_divert_fixup], [m4_divert_pop()m4_define([$0])]) m4_define([m4_init], [gl_divert_fixup()]m4_defn([m4_init])[gl_divert_fixup()])]) # AC_DEFUN_ONCE([NAME], VALUE) # ---------------------------- # Define NAME to expand to VALUE on the first use (whether by direct # expansion, or by AC_REQUIRE), and to nothing on all subsequent uses. # Avoid bugs in AC_REQUIRE in Autoconf 2.63 and earlier. This # definition is slower than the version in Autoconf 2.64, because it # can only use interfaces that existed since 2.59; but it achieves the # same effect. Quoting is necessary to avoid confusing Automake. m4_version_prereq([2.63.263], [], [m4_define([AC][_DEFUN_ONCE], [AC][_DEFUN([$1], [AC_REQUIRE([_gl_DEFUN_ONCE([$1])], [m4_indir([_gl_DEFUN_ONCE([$1])])])])]dnl [AC][_DEFUN([_gl_DEFUN_ONCE([$1])], [$2])])]) # gl_00GNULIB # ----------- # Witness macro that this file has been included. Needed to force # Automake to include this file prior to all other gnulib .m4 files. AC_DEFUN([gl_00GNULIB]) gnuastro-0.2.33-8a3b/bootstrapped/build-aux/0000755000175000017500000000000013004464723015600 500000000000000gnuastro-0.2.33-8a3b/bootstrapped/build-aux/test-driver0000755000175000017500000001104013004437004017702 00000000000000#! /bin/sh # test-driver - basic testsuite driver script. scriptversion=2013-07-13.22; # UTC # Copyright (C) 2011-2014 Free Software Foundation, Inc. # # This program is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 2, or (at your option) # any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see . # As a special exception to the GNU General Public License, if you # distribute this file as part of a program that contains a # configuration script generated by Autoconf, you may include it under # the same distribution terms that you use for the rest of that program. # This file is maintained in Automake, please report # bugs to or send patches to # . # Make unconditional expansion of undefined variables an error. This # helps a lot in preventing typo-related bugs. set -u usage_error () { echo "$0: $*" >&2 print_usage >&2 exit 2 } print_usage () { cat <$log_file 2>&1 estatus=$? if test $enable_hard_errors = no && test $estatus -eq 99; then tweaked_estatus=1 else tweaked_estatus=$estatus fi case $tweaked_estatus:$expect_failure in 0:yes) col=$red res=XPASS recheck=yes gcopy=yes;; 0:*) col=$grn res=PASS recheck=no gcopy=no;; 77:*) col=$blu res=SKIP recheck=no gcopy=yes;; 99:*) col=$mgn res=ERROR recheck=yes gcopy=yes;; *:yes) col=$lgn res=XFAIL recheck=no gcopy=yes;; *:*) col=$red res=FAIL recheck=yes gcopy=yes;; esac # Report the test outcome and exit status in the logs, so that one can # know whether the test passed or failed simply by looking at the '.log' # file, without the need of also peaking into the corresponding '.trs' # file (automake bug#11814). echo "$res $test_name (exit status: $estatus)" >>$log_file # Report outcome to console. echo "${col}${res}${std}: $test_name" # Register the test result, and other relevant metadata. echo ":test-result: $res" > $trs_file echo ":global-test-result: $res" >> $trs_file echo ":recheck: $recheck" >> $trs_file echo ":copy-in-global-log: $gcopy" >> $trs_file # Local Variables: # mode: shell-script # sh-indentation: 2 # eval: (add-hook 'write-file-hooks 'time-stamp) # time-stamp-start: "scriptversion=" # time-stamp-format: "%:y-%02m-%02d.%02H" # time-stamp-time-zone: "UTC" # time-stamp-end: "; # UTC" # End: gnuastro-0.2.33-8a3b/bootstrapped/build-aux/git-version-gen0000755000175000017500000001753413004436754020500 00000000000000#!/bin/sh # Print a version string. scriptversion=2016-05-08.18; # UTC # Copyright (C) 2007-2016 Free Software Foundation, Inc. # # This program is free software: you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see . # This script is derived from GIT-VERSION-GEN from GIT: http://git.or.cz/. # It may be run two ways: # - from a git repository in which the "git describe" command below # produces useful output (thus requiring at least one signed tag) # - from a non-git-repo directory containing a .tarball-version file, which # presumes this script is invoked like "./git-version-gen .tarball-version". # In order to use intra-version strings in your project, you will need two # separate generated version string files: # # .tarball-version - present only in a distribution tarball, and not in # a checked-out repository. Created with contents that were learned at # the last time autoconf was run, and used by git-version-gen. Must not # be present in either $(srcdir) or $(builddir) for git-version-gen to # give accurate answers during normal development with a checked out tree, # but must be present in a tarball when there is no version control system. # Therefore, it cannot be used in any dependencies. GNUmakefile has # hooks to force a reconfigure at distribution time to get the value # correct, without penalizing normal development with extra reconfigures. # # .version - present in a checked-out repository and in a distribution # tarball. Usable in dependencies, particularly for files that don't # want to depend on config.h but do want to track version changes. # Delete this file prior to any autoconf run where you want to rebuild # files to pick up a version string change; and leave it stale to # minimize rebuild time after unrelated changes to configure sources. # # As with any generated file in a VC'd directory, you should add # /.version to .gitignore, so that you don't accidentally commit it. # .tarball-version is never generated in a VC'd directory, so needn't # be listed there. # # Use the following line in your configure.ac, so that $(VERSION) will # automatically be up-to-date each time configure is run (and note that # since configure.ac no longer includes a version string, Makefile rules # should not depend on configure.ac for version updates). # # AC_INIT([GNU project], # m4_esyscmd([build-aux/git-version-gen .tarball-version]), # [bug-project@example]) # # Then use the following lines in your Makefile.am, so that .version # will be present for dependencies, and so that .version and # .tarball-version will exist in distribution tarballs. # # EXTRA_DIST = $(top_srcdir)/.version # BUILT_SOURCES = $(top_srcdir)/.version # $(top_srcdir)/.version: # echo $(VERSION) > $@-t && mv $@-t $@ # dist-hook: # echo $(VERSION) > $(distdir)/.tarball-version me=$0 version="git-version-gen $scriptversion Copyright 2011 Free Software Foundation, Inc. There is NO warranty. You may redistribute this software under the terms of the GNU General Public License. For more information about these matters, see the files named COPYING." usage="\ Usage: $me [OPTION]... \$srcdir/.tarball-version [TAG-NORMALIZATION-SED-SCRIPT] Print a version string. Options: --prefix PREFIX prefix of git tags (default 'v') --fallback VERSION fallback version to use if \"git --version\" fails --help display this help and exit --version output version information and exit Running without arguments will suffice in most cases." prefix=v fallback= while test $# -gt 0; do case $1 in --help) echo "$usage"; exit 0;; --version) echo "$version"; exit 0;; --prefix) shift; prefix=${1?};; --fallback) shift; fallback=${1?};; -*) echo "$0: Unknown option '$1'." >&2 echo "$0: Try '--help' for more information." >&2 exit 1;; *) if test "x$tarball_version_file" = x; then tarball_version_file="$1" elif test "x$tag_sed_script" = x; then tag_sed_script="$1" else echo "$0: extra non-option argument '$1'." >&2 exit 1 fi;; esac shift done if test "x$tarball_version_file" = x; then echo "$usage" exit 1 fi tag_sed_script="${tag_sed_script:-s/x/x/}" nl=' ' # Avoid meddling by environment variable of the same name. v= v_from_git= # First see if there is a tarball-only version file. # then try "git describe", then default. if test -f $tarball_version_file then v=`cat $tarball_version_file` || v= case $v in *$nl*) v= ;; # reject multi-line output [0-9]*) ;; *) v= ;; esac test "x$v" = x \ && echo "$0: WARNING: $tarball_version_file is missing or damaged" 1>&2 fi if test "x$v" != x then : # use $v # Otherwise, if there is at least one git commit involving the working # directory, and "git describe" output looks sensible, use that to # derive a version string. elif test "`git log -1 --pretty=format:x . 2>&1`" = x \ && v=`git describe --abbrev=4 --match="$prefix*" HEAD 2>/dev/null \ || git describe --abbrev=4 HEAD 2>/dev/null` \ && v=`printf '%s\n' "$v" | sed "$tag_sed_script"` \ && case $v in $prefix[0-9]*) ;; *) (exit 1) ;; esac then # Is this a new git that lists number of commits since the last # tag or the previous older version that did not? # Newer: v6.10-77-g0f8faeb # Older: v6.10-g0f8faeb case $v in *-*-*) : git describe is okay three part flavor ;; *-*) : git describe is older two part flavor # Recreate the number of commits and rewrite such that the # result is the same as if we were using the newer version # of git describe. vtag=`echo "$v" | sed 's/-.*//'` commit_list=`git rev-list "$vtag"..HEAD 2>/dev/null` \ || { commit_list=failed; echo "$0: WARNING: git rev-list failed" 1>&2; } numcommits=`echo "$commit_list" | wc -l` v=`echo "$v" | sed "s/\(.*\)-\(.*\)/\1-$numcommits-\2/"`; test "$commit_list" = failed && v=UNKNOWN ;; esac # Change the first '-' to a '.', so version-comparing tools work properly. # Remove the "g" in git describe's output string, to save a byte. v=`echo "$v" | sed 's/-/./;s/\(.*\)-g/\1-/'`; v_from_git=1 elif test "x$fallback" = x || git --version >/dev/null 2>&1; then v=UNKNOWN else v=$fallback fi v=`echo "$v" |sed "s/^$prefix//"` # Test whether to append the "-dirty" suffix only if the version # string we're using came from git. I.e., skip the test if it's "UNKNOWN" # or if it came from .tarball-version. if test "x$v_from_git" != x; then # Don't declare a version "dirty" merely because a time stamp has changed. git update-index --refresh > /dev/null 2>&1 dirty=`exec 2>/dev/null;git diff-index --name-only HEAD` || dirty= case "$dirty" in '') ;; *) # Append the suffix only if there isn't one already. case $v in *-dirty) ;; *) v="$v-dirty" ;; esac ;; esac fi # Omit the trailing newline, so that m4_esyscmd can use the result directly. printf %s "$v" # Local variables: # eval: (add-hook 'write-file-hooks 'time-stamp) # time-stamp-start: "scriptversion=" # time-stamp-format: "%:y-%02m-%02d.%02H" # time-stamp-time-zone: "UTC0" # time-stamp-end: "; # UTC" # End: gnuastro-0.2.33-8a3b/bootstrapped/build-aux/gendocs.sh0000755000175000017500000004107613004436754017514 00000000000000#!/bin/sh -e # gendocs.sh -- generate a GNU manual in many formats. This script is # mentioned in maintain.texi. See the help message below for usage details. scriptversion=2016-05-20.09 # Copyright 2003-2016 Free Software Foundation, Inc. # # This program is free software: you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see . # # Original author: Mohit Agarwal. # Send bug reports and any other correspondence to bug-gnulib@gnu.org. # # The latest version of this script, and the companion template, is # available from the Gnulib repository: # # http://git.savannah.gnu.org/cgit/gnulib.git/tree/build-aux/gendocs.sh # http://git.savannah.gnu.org/cgit/gnulib.git/tree/doc/gendocs_template # TODO: # - image importing was only implemented for HTML generated by # makeinfo. But it should be simple enough to adjust. # - images are not imported in the source tarball. All the needed # formats (PDF, PNG, etc.) should be included. prog=`basename "$0"` srcdir=`pwd` scripturl="http://git.savannah.gnu.org/cgit/gnulib.git/plain/build-aux/gendocs.sh" templateurl="http://git.savannah.gnu.org/cgit/gnulib.git/plain/doc/gendocs_template" : ${SETLANG="env LANG= LC_MESSAGES= LC_ALL= LANGUAGE="} : ${MAKEINFO="makeinfo"} : ${TEXI2DVI="texi2dvi"} : ${DOCBOOK2HTML="docbook2html"} : ${DOCBOOK2PDF="docbook2pdf"} : ${DOCBOOK2TXT="docbook2txt"} : ${GENDOCS_TEMPLATE_DIR="."} : ${PERL='perl'} : ${TEXI2HTML="texi2html"} unset CDPATH unset use_texi2html MANUAL_TITLE= PACKAGE= EMAIL=webmasters@gnu.org # please override with --email commonarg= # passed to all makeinfo/texi2html invcations. dirargs= # passed to all tools (-I dir). dirs= # -I directories. htmlarg="--css-ref=/software/gnulib/manual.css -c TOP_NODE_UP_URL=/manual" infoarg=--no-split generate_ascii=true generate_html=true generate_info=true generate_tex=true outdir=manual source_extra= split=node srcfile= texarg="-t @finalout" version="gendocs.sh $scriptversion Copyright 2016 Free Software Foundation, Inc. There is NO warranty. You may redistribute this software under the terms of the GNU General Public License. For more information about these matters, see the files named COPYING." usage="Usage: $prog [OPTION]... PACKAGE MANUAL-TITLE Generate output in various formats from PACKAGE.texinfo (or .texi or .txi) source. See the GNU Maintainers document for a more extensive discussion: http://www.gnu.org/prep/maintain_toc.html Options: --email ADR use ADR as contact in generated web pages; always give this. -s SRCFILE read Texinfo from SRCFILE, instead of PACKAGE.{texinfo|texi|txi} -o OUTDIR write files into OUTDIR, instead of manual/. -I DIR append DIR to the Texinfo search path. --common ARG pass ARG in all invocations. --html ARG pass ARG to makeinfo or texi2html for HTML targets, instead of '$htmlarg'. --info ARG pass ARG to makeinfo for Info, instead of --no-split. --no-ascii skip generating the plain text output. --no-html skip generating the html output. --no-info skip generating the info output. --no-tex skip generating the dvi and pdf output. --source ARG include ARG in tar archive of sources. --split HOW make split HTML by node, section, chapter; default node. --tex ARG pass ARG to texi2dvi for DVI and PDF, instead of -t @finalout. --texi2html use texi2html to make HTML target, with all split versions. --docbook convert through DocBook too (xml, txt, html, pdf). --help display this help and exit successfully. --version display version information and exit successfully. Simple example: $prog --email bug-gnu-emacs@gnu.org emacs \"GNU Emacs Manual\" Typical sequence: cd PACKAGESOURCE/doc wget \"$scripturl\" wget \"$templateurl\" $prog --email BUGLIST MANUAL \"GNU MANUAL - One-line description\" Output will be in a new subdirectory \"manual\" (by default; use -o OUTDIR to override). Move all the new files into your web CVS tree, as explained in the Web Pages node of maintain.texi. Please use the --email ADDRESS option so your own bug-reporting address will be used in the generated HTML pages. MANUAL-TITLE is included as part of the HTML of the overall manual/index.html file. It should include the name of the package being documented. manual/index.html is created by substitution from the file $GENDOCS_TEMPLATE_DIR/gendocs_template. (Feel free to modify the generic template for your own purposes.) If you have several manuals, you'll need to run this script several times with different MANUAL values, specifying a different output directory with -o each time. Then write (by hand) an overall index.html with links to them all. If a manual's Texinfo sources are spread across several directories, first copy or symlink all Texinfo sources into a single directory. (Part of the script's work is to make a tar.gz of the sources.) As implied above, by default monolithic Info files are generated. If you want split Info, or other Info options, use --info to override. You can set the environment variables MAKEINFO, TEXI2DVI, TEXI2HTML, and PERL to control the programs that get executed, and GENDOCS_TEMPLATE_DIR to control where the gendocs_template file is looked for. With --docbook, the environment variables DOCBOOK2HTML, DOCBOOK2PDF, and DOCBOOK2TXT are also consulted. By default, makeinfo and texi2dvi are run in the default (English) locale, since that's the language of most Texinfo manuals. If you happen to have a non-English manual and non-English web site, see the SETLANG setting in the source. Email bug reports or enhancement requests to bug-gnulib@gnu.org. " while test $# -gt 0; do case $1 in -s) shift; srcfile=$1;; -o) shift; outdir=$1;; -I) shift; dirargs="$dirargs -I '$1'"; dirs="$dirs $1";; --common) shift; commonarg=$1;; --docbook) docbook=yes;; --email) shift; EMAIL=$1;; --html) shift; htmlarg=$1;; --info) shift; infoarg=$1;; --no-ascii) generate_ascii=false;; --no-html) generate_ascii=false;; --no-info) generate_info=false;; --no-tex) generate_tex=false;; --source) shift; source_extra=$1;; --split) shift; split=$1;; --tex) shift; texarg=$1;; --texi2html) use_texi2html=1;; --help) echo "$usage"; exit 0;; --version) echo "$version"; exit 0;; -*) echo "$0: Unknown option \`$1'." >&2 echo "$0: Try \`--help' for more information." >&2 exit 1;; *) if test -z "$PACKAGE"; then PACKAGE=$1 elif test -z "$MANUAL_TITLE"; then MANUAL_TITLE=$1 else echo "$0: extra non-option argument \`$1'." >&2 exit 1 fi;; esac shift done # makeinfo uses the dirargs, but texi2dvi doesn't. commonarg=" $dirargs $commonarg" # For most of the following, the base name is just $PACKAGE base=$PACKAGE if test -n "$srcfile"; then # but here, we use the basename of $srcfile base=`basename "$srcfile"` case $base in *.txi|*.texi|*.texinfo) base=`echo "$base"|sed 's/\.[texinfo]*$//'`;; esac PACKAGE=$base elif test -s "$srcdir/$PACKAGE.texinfo"; then srcfile=$srcdir/$PACKAGE.texinfo elif test -s "$srcdir/$PACKAGE.texi"; then srcfile=$srcdir/$PACKAGE.texi elif test -s "$srcdir/$PACKAGE.txi"; then srcfile=$srcdir/$PACKAGE.txi else echo "$0: cannot find .texinfo or .texi or .txi for $PACKAGE in $srcdir." >&2 exit 1 fi if test ! -r $GENDOCS_TEMPLATE_DIR/gendocs_template; then echo "$0: cannot read $GENDOCS_TEMPLATE_DIR/gendocs_template." >&2 echo "$0: it is available from $templateurl." >&2 exit 1 fi # Function to return size of $1 in something resembling kilobytes. calcsize() { size=`ls -ksl $1 | awk '{print $1}'` echo $size } # copy_images OUTDIR HTML-FILE... # ------------------------------- # Copy all the images needed by the HTML-FILEs into OUTDIR. # Look for them in . and the -I directories; this is simpler than what # makeinfo supports with -I, but hopefully it will suffice. copy_images() { local odir odir=$1 shift $PERL -n -e " BEGIN { \$me = '$prog'; \$odir = '$odir'; @dirs = qw(. $dirs); } " -e ' /<img src="(.*?)"/g && ++$need{$1}; END { #print "$me: @{[keys %need]}\n"; # for debugging, show images found. FILE: for my $f (keys %need) { for my $d (@dirs) { if (-f "$d/$f") { use File::Basename; my $dest = dirname ("$odir/$f"); # use File::Path; -d $dest || mkpath ($dest) || die "$me: cannot mkdir $dest: $!\n"; # use File::Copy; copy ("$d/$f", $dest) || die "$me: cannot copy $d/$f to $dest: $!\n"; next FILE; } } die "$me: $ARGV: cannot find image $f\n"; } } ' -- "$@" || exit 1 } case $outdir in /*) abs_outdir=$outdir;; *) abs_outdir=$srcdir/$outdir;; esac echo "Making output for $srcfile" echo " in `pwd`" mkdir -p "$outdir/" # if $generate_info; then cmd="$SETLANG $MAKEINFO -o $PACKAGE.info $commonarg $infoarg \"$srcfile\"" echo "Generating info... ($cmd)" rm -f $PACKAGE.info* # get rid of any strays eval "$cmd" tar czf "$outdir/$PACKAGE.info.tar.gz" $PACKAGE.info* ls -l "$outdir/$PACKAGE.info.tar.gz" info_tgz_size=`calcsize "$outdir/$PACKAGE.info.tar.gz"` # do not mv the info files, there's no point in having them available # separately on the web. fi # end info # if $generate_tex; then cmd="$SETLANG $TEXI2DVI $dirargs $texarg \"$srcfile\"" printf "\nGenerating dvi... ($cmd)\n" eval "$cmd" # compress/finish dvi: gzip -f -9 $PACKAGE.dvi dvi_gz_size=`calcsize $PACKAGE.dvi.gz` mv $PACKAGE.dvi.gz "$outdir/" ls -l "$outdir/$PACKAGE.dvi.gz" cmd="$SETLANG $TEXI2DVI --pdf $dirargs $texarg \"$srcfile\"" printf "\nGenerating pdf... ($cmd)\n" eval "$cmd" pdf_size=`calcsize $PACKAGE.pdf` mv $PACKAGE.pdf "$outdir/" ls -l "$outdir/$PACKAGE.pdf" fi # end tex (dvi + pdf) # if $generate_ascii; then opt="-o $PACKAGE.txt --no-split --no-headers $commonarg" cmd="$SETLANG $MAKEINFO $opt \"$srcfile\"" printf "\nGenerating ascii... ($cmd)\n" eval "$cmd" ascii_size=`calcsize $PACKAGE.txt` gzip -f -9 -c $PACKAGE.txt >"$outdir/$PACKAGE.txt.gz" ascii_gz_size=`calcsize "$outdir/$PACKAGE.txt.gz"` mv $PACKAGE.txt "$outdir/" ls -l "$outdir/$PACKAGE.txt" "$outdir/$PACKAGE.txt.gz" fi # if $generate_html; then # Split HTML at level $1. Used for texi2html. html_split() { opt="--split=$1 --node-files $commonarg $htmlarg" cmd="$SETLANG $TEXI2HTML --output $PACKAGE.html $opt \"$srcfile\"" printf "\nGenerating html by $1... ($cmd)\n" eval "$cmd" split_html_dir=$PACKAGE.html ( cd ${split_html_dir} || exit 1 ln -sf ${PACKAGE}.html index.html tar -czf "$abs_outdir/${PACKAGE}.html_$1.tar.gz" -- *.html ) eval html_$1_tgz_size=`calcsize "$outdir/${PACKAGE}.html_$1.tar.gz"` rm -f "$outdir"/html_$1/*.html mkdir -p "$outdir/html_$1/" mv ${split_html_dir}/*.html "$outdir/html_$1/" rmdir ${split_html_dir} } if test -z "$use_texi2html"; then opt="--no-split --html -o $PACKAGE.html $commonarg $htmlarg" cmd="$SETLANG $MAKEINFO $opt \"$srcfile\"" printf "\nGenerating monolithic html... ($cmd)\n" rm -rf $PACKAGE.html # in case a directory is left over eval "$cmd" html_mono_size=`calcsize $PACKAGE.html` gzip -f -9 -c $PACKAGE.html >"$outdir/$PACKAGE.html.gz" html_mono_gz_size=`calcsize "$outdir/$PACKAGE.html.gz"` copy_images "$outdir/" $PACKAGE.html mv $PACKAGE.html "$outdir/" ls -l "$outdir/$PACKAGE.html" "$outdir/$PACKAGE.html.gz" # Before Texinfo 5.0, makeinfo did not accept a --split=HOW option, # it just always split by node. So if we're splitting by node anyway, # leave it out. if test "x$split" = xnode; then split_arg= else split_arg=--split=$split fi # opt="--html -o $PACKAGE.html $split_arg $commonarg $htmlarg" cmd="$SETLANG $MAKEINFO $opt \"$srcfile\"" printf "\nGenerating html by $split... ($cmd)\n" eval "$cmd" split_html_dir=$PACKAGE.html copy_images $split_html_dir/ $split_html_dir/*.html ( cd $split_html_dir || exit 1 tar -czf "$abs_outdir/$PACKAGE.html_$split.tar.gz" -- * ) eval \ html_${split}_tgz_size=`calcsize "$outdir/$PACKAGE.html_$split.tar.gz"` rm -rf "$outdir/html_$split/" mv $split_html_dir "$outdir/html_$split/" du -s "$outdir/html_$split/" ls -l "$outdir/$PACKAGE.html_$split.tar.gz" else # use texi2html: opt="--output $PACKAGE.html $commonarg $htmlarg" cmd="$SETLANG $TEXI2HTML $opt \"$srcfile\"" printf "\nGenerating monolithic html with texi2html... ($cmd)\n" rm -rf $PACKAGE.html # in case a directory is left over eval "$cmd" html_mono_size=`calcsize $PACKAGE.html` gzip -f -9 -c $PACKAGE.html >"$outdir/$PACKAGE.html.gz" html_mono_gz_size=`calcsize "$outdir/$PACKAGE.html.gz"` mv $PACKAGE.html "$outdir/" html_split node html_split chapter html_split section fi fi # end html # printf "\nMaking .tar.gz for sources...\n" d=`dirname $srcfile` ( cd "$d" srcfiles=`ls -d *.texinfo *.texi *.txi *.eps $source_extra 2>/dev/null` || true tar czfh "$abs_outdir/$PACKAGE.texi.tar.gz" $srcfiles ls -l "$abs_outdir/$PACKAGE.texi.tar.gz" ) texi_tgz_size=`calcsize "$outdir/$PACKAGE.texi.tar.gz"` # # Do everything again through docbook. if test -n "$docbook"; then opt="-o - --docbook $commonarg" cmd="$SETLANG $MAKEINFO $opt \"$srcfile\" >${srcdir}/$PACKAGE-db.xml" printf "\nGenerating docbook XML... ($cmd)\n" eval "$cmd" docbook_xml_size=`calcsize $PACKAGE-db.xml` gzip -f -9 -c $PACKAGE-db.xml >"$outdir/$PACKAGE-db.xml.gz" docbook_xml_gz_size=`calcsize "$outdir/$PACKAGE-db.xml.gz"` mv $PACKAGE-db.xml "$outdir/" split_html_db_dir=html_node_db opt="$commonarg -o $split_html_db_dir" cmd="$DOCBOOK2HTML $opt \"${outdir}/$PACKAGE-db.xml\"" printf "\nGenerating docbook HTML... ($cmd)\n" eval "$cmd" ( cd ${split_html_db_dir} || exit 1 tar -czf "$abs_outdir/${PACKAGE}.html_node_db.tar.gz" -- *.html ) html_node_db_tgz_size=`calcsize "$outdir/${PACKAGE}.html_node_db.tar.gz"` rm -f "$outdir"/html_node_db/*.html mkdir -p "$outdir/html_node_db" mv ${split_html_db_dir}/*.html "$outdir/html_node_db/" rmdir ${split_html_db_dir} cmd="$DOCBOOK2TXT \"${outdir}/$PACKAGE-db.xml\"" printf "\nGenerating docbook ASCII... ($cmd)\n" eval "$cmd" docbook_ascii_size=`calcsize $PACKAGE-db.txt` mv $PACKAGE-db.txt "$outdir/" cmd="$DOCBOOK2PDF \"${outdir}/$PACKAGE-db.xml\"" printf "\nGenerating docbook PDF... ($cmd)\n" eval "$cmd" docbook_pdf_size=`calcsize $PACKAGE-db.pdf` mv $PACKAGE-db.pdf "$outdir/" fi # printf "\nMaking index.html for $PACKAGE...\n" if test -z "$use_texi2html"; then CONDS="/%%IF *HTML_SECTION%%/,/%%ENDIF *HTML_SECTION%%/d;\ /%%IF *HTML_CHAPTER%%/,/%%ENDIF *HTML_CHAPTER%%/d" else # should take account of --split here. CONDS="/%%ENDIF.*%%/d;/%%IF *HTML_SECTION%%/d;/%%IF *HTML_CHAPTER%%/d" fi curdate=`$SETLANG date '+%B %d, %Y'` sed \ -e "s!%%TITLE%%!$MANUAL_TITLE!g" \ -e "s!%%EMAIL%%!$EMAIL!g" \ -e "s!%%PACKAGE%%!$PACKAGE!g" \ -e "s!%%DATE%%!$curdate!g" \ -e "s!%%HTML_MONO_SIZE%%!$html_mono_size!g" \ -e "s!%%HTML_MONO_GZ_SIZE%%!$html_mono_gz_size!g" \ -e "s!%%HTML_NODE_TGZ_SIZE%%!$html_node_tgz_size!g" \ -e "s!%%HTML_SECTION_TGZ_SIZE%%!$html_section_tgz_size!g" \ -e "s!%%HTML_CHAPTER_TGZ_SIZE%%!$html_chapter_tgz_size!g" \ -e "s!%%INFO_TGZ_SIZE%%!$info_tgz_size!g" \ -e "s!%%DVI_GZ_SIZE%%!$dvi_gz_size!g" \ -e "s!%%PDF_SIZE%%!$pdf_size!g" \ -e "s!%%ASCII_SIZE%%!$ascii_size!g" \ -e "s!%%ASCII_GZ_SIZE%%!$ascii_gz_size!g" \ -e "s!%%TEXI_TGZ_SIZE%%!$texi_tgz_size!g" \ -e "s!%%DOCBOOK_HTML_NODE_TGZ_SIZE%%!$html_node_db_tgz_size!g" \ -e "s!%%DOCBOOK_ASCII_SIZE%%!$docbook_ascii_size!g" \ -e "s!%%DOCBOOK_PDF_SIZE%%!$docbook_pdf_size!g" \ -e "s!%%DOCBOOK_XML_SIZE%%!$docbook_xml_size!g" \ -e "s!%%DOCBOOK_XML_GZ_SIZE%%!$docbook_xml_gz_size!g" \ -e "s,%%SCRIPTURL%%,$scripturl,g" \ -e "s!%%SCRIPTNAME%%!$prog!g" \ -e "$CONDS" \ $GENDOCS_TEMPLATE_DIR/gendocs_template >"$outdir/index.html" echo "Done, see $outdir/ subdirectory for new files." # Local variables: # eval: (add-hook 'write-file-hooks 'time-stamp) # time-stamp-start: "scriptversion=" # time-stamp-format: "%:y-%02m-%02d.%02H" # time-stamp-end: "$" # End: ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.2.33-8a3b/bootstrapped/build-aux/snippet/������������������������������������������������0000755�0001750�0001750�00000000000�13004464723�017262� 5����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.2.33-8a3b/bootstrapped/build-aux/snippet/warn-on-use.h�����������������������������������0000644�0001750�0001750�00000012007�13004436754�021531� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/* A C macro for emitting warnings if a function is used. Copyright (C) 2010-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see <http://www.gnu.org/licenses/>. */ /* _GL_WARN_ON_USE (function, "literal string") issues a declaration for FUNCTION which will then trigger a compiler warning containing the text of "literal string" anywhere that function is called, if supported by the compiler. If the compiler does not support this feature, the macro expands to an unused extern declaration. This macro is useful for marking a function as a potential portability trap, with the intent that "literal string" include instructions on the replacement function that should be used instead. However, one of the reasons that a function is a portability trap is if it has the wrong signature. Declaring FUNCTION with a different signature in C is a compilation error, so this macro must use the same type as any existing declaration so that programs that avoid the problematic FUNCTION do not fail to compile merely because they included a header that poisoned the function. But this implies that _GL_WARN_ON_USE is only safe to use if FUNCTION is known to already have a declaration. Use of this macro implies that there must not be any other macro hiding the declaration of FUNCTION; but undefining FUNCTION first is part of the poisoning process anyway (although for symbols that are provided only via a macro, the result is a compilation error rather than a warning containing "literal string"). Also note that in C++, it is only safe to use if FUNCTION has no overloads. For an example, it is possible to poison 'getline' by: - adding a call to gl_WARN_ON_USE_PREPARE([[#include <stdio.h>]], [getline]) in configure.ac, which potentially defines HAVE_RAW_DECL_GETLINE - adding this code to a header that wraps the system <stdio.h>: #undef getline #if HAVE_RAW_DECL_GETLINE _GL_WARN_ON_USE (getline, "getline is required by POSIX 2008, but" "not universally present; use the gnulib module getline"); #endif It is not possible to directly poison global variables. But it is possible to write a wrapper accessor function, and poison that (less common usage, like &environ, will cause a compilation error rather than issue the nice warning, but the end result of informing the developer about their portability problem is still achieved): #if HAVE_RAW_DECL_ENVIRON static char ***rpl_environ (void) { return &environ; } _GL_WARN_ON_USE (rpl_environ, "environ is not always properly declared"); # undef environ # define environ (*rpl_environ ()) #endif */ #ifndef _GL_WARN_ON_USE # if 4 < __GNUC__ || (__GNUC__ == 4 && 3 <= __GNUC_MINOR__) /* A compiler attribute is available in gcc versions 4.3.0 and later. */ # define _GL_WARN_ON_USE(function, message) \ extern __typeof__ (function) function __attribute__ ((__warning__ (message))) # elif __GNUC__ >= 3 && GNULIB_STRICT_CHECKING /* Verify the existence of the function. */ # define _GL_WARN_ON_USE(function, message) \ extern __typeof__ (function) function # else /* Unsupported. */ # define _GL_WARN_ON_USE(function, message) \ _GL_WARN_EXTERN_C int _gl_warn_on_use # endif #endif /* _GL_WARN_ON_USE_CXX (function, rettype, parameters_and_attributes, "string") is like _GL_WARN_ON_USE (function, "string"), except that the function is declared with the given prototype, consisting of return type, parameters, and attributes. This variant is useful for overloaded functions in C++. _GL_WARN_ON_USE does not work in this case. */ #ifndef _GL_WARN_ON_USE_CXX # if 4 < __GNUC__ || (__GNUC__ == 4 && 3 <= __GNUC_MINOR__) # define _GL_WARN_ON_USE_CXX(function,rettype,parameters_and_attributes,msg) \ extern rettype function parameters_and_attributes \ __attribute__ ((__warning__ (msg))) # elif __GNUC__ >= 3 && GNULIB_STRICT_CHECKING /* Verify the existence of the function. */ # define _GL_WARN_ON_USE_CXX(function,rettype,parameters_and_attributes,msg) \ extern rettype function parameters_and_attributes # else /* Unsupported. */ # define _GL_WARN_ON_USE_CXX(function,rettype,parameters_and_attributes,msg) \ _GL_WARN_EXTERN_C int _gl_warn_on_use # endif #endif /* _GL_WARN_EXTERN_C declaration; performs the declaration with C linkage. */ #ifndef _GL_WARN_EXTERN_C # if defined __cplusplus # define _GL_WARN_EXTERN_C extern "C" # else # define _GL_WARN_EXTERN_C extern # endif #endif �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.2.33-8a3b/bootstrapped/build-aux/snippet/c++defs.h���������������������������������������0000644�0001750�0001750�00000026753�13004436754�020605� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/* C++ compatible function declaration macros. Copyright (C) 2010-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see <http://www.gnu.org/licenses/>. */ #ifndef _GL_CXXDEFS_H #define _GL_CXXDEFS_H /* The three most frequent use cases of these macros are: * For providing a substitute for a function that is missing on some platforms, but is declared and works fine on the platforms on which it exists: #if @GNULIB_FOO@ # if !@HAVE_FOO@ _GL_FUNCDECL_SYS (foo, ...); # endif _GL_CXXALIAS_SYS (foo, ...); _GL_CXXALIASWARN (foo); #elif defined GNULIB_POSIXCHECK ... #endif * For providing a replacement for a function that exists on all platforms, but is broken/insufficient and needs to be replaced on some platforms: #if @GNULIB_FOO@ # if @REPLACE_FOO@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef foo # define foo rpl_foo # endif _GL_FUNCDECL_RPL (foo, ...); _GL_CXXALIAS_RPL (foo, ...); # else _GL_CXXALIAS_SYS (foo, ...); # endif _GL_CXXALIASWARN (foo); #elif defined GNULIB_POSIXCHECK ... #endif * For providing a replacement for a function that exists on some platforms but is broken/insufficient and needs to be replaced on some of them and is additionally either missing or undeclared on some other platforms: #if @GNULIB_FOO@ # if @REPLACE_FOO@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef foo # define foo rpl_foo # endif _GL_FUNCDECL_RPL (foo, ...); _GL_CXXALIAS_RPL (foo, ...); # else # if !@HAVE_FOO@ or if !@HAVE_DECL_FOO@ _GL_FUNCDECL_SYS (foo, ...); # endif _GL_CXXALIAS_SYS (foo, ...); # endif _GL_CXXALIASWARN (foo); #elif defined GNULIB_POSIXCHECK ... #endif */ /* _GL_EXTERN_C declaration; performs the declaration with C linkage. */ #if defined __cplusplus # define _GL_EXTERN_C extern "C" #else # define _GL_EXTERN_C extern #endif /* _GL_FUNCDECL_RPL (func, rettype, parameters_and_attributes); declares a replacement function, named rpl_func, with the given prototype, consisting of return type, parameters, and attributes. Example: _GL_FUNCDECL_RPL (open, int, (const char *filename, int flags, ...) _GL_ARG_NONNULL ((1))); */ #define _GL_FUNCDECL_RPL(func,rettype,parameters_and_attributes) \ _GL_FUNCDECL_RPL_1 (rpl_##func, rettype, parameters_and_attributes) #define _GL_FUNCDECL_RPL_1(rpl_func,rettype,parameters_and_attributes) \ _GL_EXTERN_C rettype rpl_func parameters_and_attributes /* _GL_FUNCDECL_SYS (func, rettype, parameters_and_attributes); declares the system function, named func, with the given prototype, consisting of return type, parameters, and attributes. Example: _GL_FUNCDECL_SYS (open, int, (const char *filename, int flags, ...) _GL_ARG_NONNULL ((1))); */ #define _GL_FUNCDECL_SYS(func,rettype,parameters_and_attributes) \ _GL_EXTERN_C rettype func parameters_and_attributes /* _GL_CXXALIAS_RPL (func, rettype, parameters); declares a C++ alias called GNULIB_NAMESPACE::func that redirects to rpl_func, if GNULIB_NAMESPACE is defined. Example: _GL_CXXALIAS_RPL (open, int, (const char *filename, int flags, ...)); */ #define _GL_CXXALIAS_RPL(func,rettype,parameters) \ _GL_CXXALIAS_RPL_1 (func, rpl_##func, rettype, parameters) #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIAS_RPL_1(func,rpl_func,rettype,parameters) \ namespace GNULIB_NAMESPACE \ { \ rettype (*const func) parameters = ::rpl_func; \ } \ _GL_EXTERN_C int _gl_cxxalias_dummy #else # define _GL_CXXALIAS_RPL_1(func,rpl_func,rettype,parameters) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIAS_RPL_CAST_1 (func, rpl_func, rettype, parameters); is like _GL_CXXALIAS_RPL_1 (func, rpl_func, rettype, parameters); except that the C function rpl_func may have a slightly different declaration. A cast is used to silence the "invalid conversion" error that would otherwise occur. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIAS_RPL_CAST_1(func,rpl_func,rettype,parameters) \ namespace GNULIB_NAMESPACE \ { \ rettype (*const func) parameters = \ reinterpret_cast<rettype(*)parameters>(::rpl_func); \ } \ _GL_EXTERN_C int _gl_cxxalias_dummy #else # define _GL_CXXALIAS_RPL_CAST_1(func,rpl_func,rettype,parameters) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIAS_SYS (func, rettype, parameters); declares a C++ alias called GNULIB_NAMESPACE::func that redirects to the system provided function func, if GNULIB_NAMESPACE is defined. Example: _GL_CXXALIAS_SYS (open, int, (const char *filename, int flags, ...)); */ #if defined __cplusplus && defined GNULIB_NAMESPACE /* If we were to write rettype (*const func) parameters = ::func; like above in _GL_CXXALIAS_RPL_1, the compiler could optimize calls better (remove an indirection through a 'static' pointer variable), but then the _GL_CXXALIASWARN macro below would cause a warning not only for uses of ::func but also for uses of GNULIB_NAMESPACE::func. */ # define _GL_CXXALIAS_SYS(func,rettype,parameters) \ namespace GNULIB_NAMESPACE \ { \ static rettype (*func) parameters = ::func; \ } \ _GL_EXTERN_C int _gl_cxxalias_dummy #else # define _GL_CXXALIAS_SYS(func,rettype,parameters) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIAS_SYS_CAST (func, rettype, parameters); is like _GL_CXXALIAS_SYS (func, rettype, parameters); except that the C function func may have a slightly different declaration. A cast is used to silence the "invalid conversion" error that would otherwise occur. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIAS_SYS_CAST(func,rettype,parameters) \ namespace GNULIB_NAMESPACE \ { \ static rettype (*func) parameters = \ reinterpret_cast<rettype(*)parameters>(::func); \ } \ _GL_EXTERN_C int _gl_cxxalias_dummy #else # define _GL_CXXALIAS_SYS_CAST(func,rettype,parameters) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIAS_SYS_CAST2 (func, rettype, parameters, rettype2, parameters2); is like _GL_CXXALIAS_SYS (func, rettype, parameters); except that the C function is picked among a set of overloaded functions, namely the one with rettype2 and parameters2. Two consecutive casts are used to silence the "cannot find a match" and "invalid conversion" errors that would otherwise occur. */ #if defined __cplusplus && defined GNULIB_NAMESPACE /* The outer cast must be a reinterpret_cast. The inner cast: When the function is defined as a set of overloaded functions, it works as a static_cast<>, choosing the designated variant. When the function is defined as a single variant, it works as a reinterpret_cast<>. The parenthesized cast syntax works both ways. */ # define _GL_CXXALIAS_SYS_CAST2(func,rettype,parameters,rettype2,parameters2) \ namespace GNULIB_NAMESPACE \ { \ static rettype (*func) parameters = \ reinterpret_cast<rettype(*)parameters>( \ (rettype2(*)parameters2)(::func)); \ } \ _GL_EXTERN_C int _gl_cxxalias_dummy #else # define _GL_CXXALIAS_SYS_CAST2(func,rettype,parameters,rettype2,parameters2) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIASWARN (func); causes a warning to be emitted when ::func is used but not when GNULIB_NAMESPACE::func is used. func must be defined without overloaded variants. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIASWARN(func) \ _GL_CXXALIASWARN_1 (func, GNULIB_NAMESPACE) # define _GL_CXXALIASWARN_1(func,namespace) \ _GL_CXXALIASWARN_2 (func, namespace) /* To work around GCC bug <http://gcc.gnu.org/bugzilla/show_bug.cgi?id=43881>, we enable the warning only when not optimizing. */ # if !__OPTIMIZE__ # define _GL_CXXALIASWARN_2(func,namespace) \ _GL_WARN_ON_USE (func, \ "The symbol ::" #func " refers to the system function. " \ "Use " #namespace "::" #func " instead.") # elif __GNUC__ >= 3 && GNULIB_STRICT_CHECKING # define _GL_CXXALIASWARN_2(func,namespace) \ extern __typeof__ (func) func # else # define _GL_CXXALIASWARN_2(func,namespace) \ _GL_EXTERN_C int _gl_cxxalias_dummy # endif #else # define _GL_CXXALIASWARN(func) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIASWARN1 (func, rettype, parameters_and_attributes); causes a warning to be emitted when the given overloaded variant of ::func is used but not when GNULIB_NAMESPACE::func is used. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIASWARN1(func,rettype,parameters_and_attributes) \ _GL_CXXALIASWARN1_1 (func, rettype, parameters_and_attributes, \ GNULIB_NAMESPACE) # define _GL_CXXALIASWARN1_1(func,rettype,parameters_and_attributes,namespace) \ _GL_CXXALIASWARN1_2 (func, rettype, parameters_and_attributes, namespace) /* To work around GCC bug <http://gcc.gnu.org/bugzilla/show_bug.cgi?id=43881>, we enable the warning only when not optimizing. */ # if !__OPTIMIZE__ # define _GL_CXXALIASWARN1_2(func,rettype,parameters_and_attributes,namespace) \ _GL_WARN_ON_USE_CXX (func, rettype, parameters_and_attributes, \ "The symbol ::" #func " refers to the system function. " \ "Use " #namespace "::" #func " instead.") # elif __GNUC__ >= 3 && GNULIB_STRICT_CHECKING # define _GL_CXXALIASWARN1_2(func,rettype,parameters_and_attributes,namespace) \ extern __typeof__ (func) func # else # define _GL_CXXALIASWARN1_2(func,rettype,parameters_and_attributes,namespace) \ _GL_EXTERN_C int _gl_cxxalias_dummy # endif #else # define _GL_CXXALIASWARN1(func,rettype,parameters_and_attributes) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif #endif /* _GL_CXXDEFS_H */ ���������������������gnuastro-0.2.33-8a3b/bootstrapped/build-aux/snippet/arg-nonnull.h�����������������������������������0000644�0001750�0001750�00000002300�13004436754�021605� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/* A C macro for declaring that specific arguments must not be NULL. Copyright (C) 2009-2016 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see <http://www.gnu.org/licenses/>. */ /* _GL_ARG_NONNULL((n,...,m)) tells the compiler and static analyzer tools that the values passed as arguments n, ..., m must be non-NULL pointers. n = 1 stands for the first argument, n = 2 for the second argument etc. */ #ifndef _GL_ARG_NONNULL # if (__GNUC__ == 3 && __GNUC_MINOR__ >= 3) || __GNUC__ > 3 # define _GL_ARG_NONNULL(params) __attribute__ ((__nonnull__ params)) # else # define _GL_ARG_NONNULL(params) # endif #endif ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.2.33-8a3b/bootstrapped/build-aux/snippet/_Noreturn.h�������������������������������������0000644�0001750�0001750�00000000462�13004436754�021333� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������#if !defined _Noreturn && __STDC_VERSION__ < 201112 # if (3 <= __GNUC__ || (__GNUC__ == 2 && 8 <= __GNUC_MINOR__) \ || 0x5110 <= __SUNPRO_C) # define _Noreturn __attribute__ ((__noreturn__)) # elif 1200 <= _MSC_VER # define _Noreturn __declspec (noreturn) # else # define _Noreturn # endif #endif ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.2.33-8a3b/bootstrapped/build-aux/texinfo.tex���������������������������������������������0000644�0001750�0001750�00001347506�12770606474�017750� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������% texinfo.tex -- TeX macros to handle Texinfo files. % % Load plain if necessary, i.e., if running under initex. \expandafter\ifx\csname fmtname\endcsname\relax\input plain\fi % \def\texinfoversion{2016-09-18.18} % % Copyright 1985, 1986, 1988, 1990, 1991, 1992, 1993, 1994, 1995, % 1996, 1997, 1998, 1999, 2000, 2001, 2002, 2003, 2004, 2005, 2006, % 2007, 2008, 2009, 2010, 2011, 2012, 2013, 2014, 2015, 2016 % Free Software Foundation, Inc. % % This texinfo.tex file is free software: you can redistribute it and/or % modify it under the terms of the GNU General Public License as % published by the Free Software Foundation, either version 3 of the % License, or (at your option) any later version. % % This texinfo.tex file is distributed in the hope that it will be % useful, but WITHOUT ANY WARRANTY; without even the implied warranty % of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU % General Public License for more details. % % You should have received a copy of the GNU General Public License % along with this program. If not, see <http://www.gnu.org/licenses/>. % % As a special exception, when this file is read by TeX when processing % a Texinfo source document, you may use the result without % restriction. This Exception is an additional permission under section 7 % of the GNU General Public License, version 3 ("GPLv3"). % % Please try the latest version of texinfo.tex before submitting bug % reports; you can get the latest version from: % http://ftp.gnu.org/gnu/texinfo/ (the Texinfo release area), or % http://ftpmirror.gnu.org/texinfo/ (same, via a mirror), or % http://www.gnu.org/software/texinfo/ (the Texinfo home page) % The texinfo.tex in any given distribution could well be out % of date, so if that's what you're using, please check. % % Send bug reports to bug-texinfo@gnu.org. Please include including a % complete document in each bug report with which we can reproduce the % problem. Patches are, of course, greatly appreciated. % % To process a Texinfo manual with TeX, it's most reliable to use the % texi2dvi shell script that comes with the distribution. For a simple % manual foo.texi, however, you can get away with this: % tex foo.texi % texindex foo.?? % tex foo.texi % tex foo.texi % dvips foo.dvi -o # or whatever; this makes foo.ps. % The extra TeX runs get the cross-reference information correct. % Sometimes one run after texindex suffices, and sometimes you need more % than two; texi2dvi does it as many times as necessary. % % It is possible to adapt texinfo.tex for other languages, to some % extent. You can get the existing language-specific files from the % full Texinfo distribution. % % The GNU Texinfo home page is http://www.gnu.org/software/texinfo. \message{Loading texinfo [version \texinfoversion]:} % If in a .fmt file, print the version number % and turn on active characters that we couldn't do earlier because % they might have appeared in the input file name. \everyjob{\message{[Texinfo version \texinfoversion]}% \catcode`+=\active \catcode`\_=\active} % LaTeX's \typeout. This ensures that the messages it is used for % are identical in format to the corresponding ones from latex/pdflatex. \def\typeout{\immediate\write17}% \chardef\other=12 % We never want plain's \outer definition of \+ in Texinfo. % For @tex, we can use \tabalign. \let\+ = \relax % Save some plain tex macros whose names we will redefine. \let\ptexb=\b \let\ptexbullet=\bullet \let\ptexc=\c \let\ptexcomma=\, \let\ptexdot=\. \let\ptexdots=\dots \let\ptexend=\end \let\ptexequiv=\equiv \let\ptexexclam=\! \let\ptexfootnote=\footnote \let\ptexgtr=> \let\ptexhat=^ \let\ptexi=\i \let\ptexindent=\indent \let\ptexinsert=\insert \let\ptexlbrace=\{ \let\ptexless=< \let\ptexnewwrite\newwrite \let\ptexnoindent=\noindent \let\ptexplus=+ \let\ptexraggedright=\raggedright \let\ptexrbrace=\} \let\ptexslash=\/ \let\ptexsp=\sp \let\ptexstar=\* \let\ptexsup=\sup \let\ptext=\t \let\ptextop=\top {\catcode`\'=\active \global\let\ptexquoteright'}% active in plain's math mode % If this character appears in an error message or help string, it % starts a new line in the output. \newlinechar = `^^J % Use TeX 3.0's \inputlineno to get the line number, for better error % messages, but if we're using an old version of TeX, don't do anything. % \ifx\inputlineno\thisisundefined \let\linenumber = \empty % Pre-3.0. \else \def\linenumber{l.\the\inputlineno:\space} \fi % Set up fixed words for English if not already set. \ifx\putwordAppendix\undefined \gdef\putwordAppendix{Appendix}\fi \ifx\putwordChapter\undefined \gdef\putwordChapter{Chapter}\fi \ifx\putworderror\undefined \gdef\putworderror{error}\fi \ifx\putwordfile\undefined \gdef\putwordfile{file}\fi \ifx\putwordin\undefined \gdef\putwordin{in}\fi \ifx\putwordIndexIsEmpty\undefined \gdef\putwordIndexIsEmpty{(Index is empty)}\fi \ifx\putwordIndexNonexistent\undefined \gdef\putwordIndexNonexistent{(Index is nonexistent)}\fi \ifx\putwordInfo\undefined \gdef\putwordInfo{Info}\fi \ifx\putwordInstanceVariableof\undefined \gdef\putwordInstanceVariableof{Instance Variable of}\fi \ifx\putwordMethodon\undefined \gdef\putwordMethodon{Method on}\fi \ifx\putwordNoTitle\undefined \gdef\putwordNoTitle{No Title}\fi \ifx\putwordof\undefined \gdef\putwordof{of}\fi \ifx\putwordon\undefined \gdef\putwordon{on}\fi \ifx\putwordpage\undefined \gdef\putwordpage{page}\fi \ifx\putwordsection\undefined \gdef\putwordsection{section}\fi \ifx\putwordSection\undefined \gdef\putwordSection{Section}\fi \ifx\putwordsee\undefined \gdef\putwordsee{see}\fi \ifx\putwordSee\undefined \gdef\putwordSee{See}\fi \ifx\putwordShortTOC\undefined \gdef\putwordShortTOC{Short Contents}\fi \ifx\putwordTOC\undefined \gdef\putwordTOC{Table of Contents}\fi % \ifx\putwordMJan\undefined \gdef\putwordMJan{January}\fi \ifx\putwordMFeb\undefined \gdef\putwordMFeb{February}\fi \ifx\putwordMMar\undefined \gdef\putwordMMar{March}\fi \ifx\putwordMApr\undefined \gdef\putwordMApr{April}\fi \ifx\putwordMMay\undefined \gdef\putwordMMay{May}\fi \ifx\putwordMJun\undefined \gdef\putwordMJun{June}\fi \ifx\putwordMJul\undefined \gdef\putwordMJul{July}\fi \ifx\putwordMAug\undefined \gdef\putwordMAug{August}\fi \ifx\putwordMSep\undefined \gdef\putwordMSep{September}\fi \ifx\putwordMOct\undefined \gdef\putwordMOct{October}\fi \ifx\putwordMNov\undefined \gdef\putwordMNov{November}\fi \ifx\putwordMDec\undefined \gdef\putwordMDec{December}\fi % \ifx\putwordDefmac\undefined \gdef\putwordDefmac{Macro}\fi \ifx\putwordDefspec\undefined \gdef\putwordDefspec{Special Form}\fi \ifx\putwordDefvar\undefined \gdef\putwordDefvar{Variable}\fi \ifx\putwordDefopt\undefined \gdef\putwordDefopt{User Option}\fi \ifx\putwordDeffunc\undefined \gdef\putwordDeffunc{Function}\fi % Give the space character the catcode for a space. \def\spaceisspace{\catcode`\ =10\relax} \chardef\dashChar = `\- \chardef\slashChar = `\/ \chardef\underChar = `\_ % Ignore a token. % \def\gobble#1{} % The following is used inside several \edef's. \def\makecsname#1{\expandafter\noexpand\csname#1\endcsname} % Hyphenation fixes. \hyphenation{ Flor-i-da Ghost-script Ghost-view Mac-OS Post-Script ap-pen-dix bit-map bit-maps data-base data-bases eshell fall-ing half-way long-est man-u-script man-u-scripts mini-buf-fer mini-buf-fers over-view par-a-digm par-a-digms rath-er rec-tan-gu-lar ro-bot-ics se-vere-ly set-up spa-ces spell-ing spell-ings stand-alone strong-est time-stamp time-stamps which-ever white-space wide-spread wrap-around } % Sometimes it is convenient to have everything in the transcript file % and nothing on the terminal. We don't just call \tracingall here, % since that produces some useless output on the terminal. We also make % some effort to order the tracing commands to reduce output in the log % file; cf. trace.sty in LaTeX. % \def\gloggingall{\begingroup \globaldefs = 1 \loggingall \endgroup}% \def\loggingall{% \tracingstats2 \tracingpages1 \tracinglostchars2 % 2 gives us more in etex \tracingparagraphs1 \tracingoutput1 \tracingmacros2 \tracingrestores1 \showboxbreadth\maxdimen \showboxdepth\maxdimen \ifx\eTeXversion\thisisundefined\else % etex gives us more logging \tracingscantokens1 \tracingifs1 \tracinggroups1 \tracingnesting2 \tracingassigns1 \fi \tracingcommands3 % 3 gives us more in etex \errorcontextlines16 }% % @errormsg{MSG}. Do the index-like expansions on MSG, but if things % aren't perfect, it's not the end of the world, being an error message, % after all. % \def\errormsg{\begingroup \indexnofonts \doerrormsg} \def\doerrormsg#1{\errmessage{#1}} % add check for \lastpenalty to plain's definitions. If the last thing % we did was a \nobreak, we don't want to insert more space. % \def\smallbreak{\ifnum\lastpenalty<10000\par\ifdim\lastskip<\smallskipamount \removelastskip\penalty-50\smallskip\fi\fi} \def\medbreak{\ifnum\lastpenalty<10000\par\ifdim\lastskip<\medskipamount \removelastskip\penalty-100\medskip\fi\fi} \def\bigbreak{\ifnum\lastpenalty<10000\par\ifdim\lastskip<\bigskipamount \removelastskip\penalty-200\bigskip\fi\fi} % Output routine % % For a final copy, take out the rectangles % that mark overfull boxes (in case you have decided % that the text looks ok even though it passes the margin). % \def\finalout{\overfullrule=0pt } % Do @cropmarks to get crop marks. % \newif\ifcropmarks \let\cropmarks = \cropmarkstrue % % Dimensions to add cropmarks at corners. % Added by P. A. MacKay, 12 Nov. 1986 % \newdimen\outerhsize \newdimen\outervsize % set by the paper size routines \newdimen\cornerlong \cornerlong=1pc \newdimen\cornerthick \cornerthick=.3pt \newdimen\topandbottommargin \topandbottommargin=.75in % Output a mark which sets \thischapter, \thissection and \thiscolor. % We dump everything together because we only have one kind of mark. % This works because we only use \botmark / \topmark, not \firstmark. % % A mark contains a subexpression of the \ifcase ... \fi construct. % \get*marks macros below extract the needed part using \ifcase. % % Another complication is to let the user choose whether \thischapter % (\thissection) refers to the chapter (section) in effect at the top % of a page, or that at the bottom of a page. % \domark is called twice inside \chapmacro, to add one % mark before the section break, and one after. % In the second call \prevchapterdefs is the same as \lastchapterdefs, % and \prevsectiondefs is the same as \lastsectiondefs. % Then if the page is not broken at the mark, some of the previous % section appears on the page, and we can get the name of this section % from \firstmark for @everyheadingmarks top. % @everyheadingmarks bottom uses \botmark. % % See page 260 of The TeXbook. \def\domark{% \toks0=\expandafter{\lastchapterdefs}% \toks2=\expandafter{\lastsectiondefs}% \toks4=\expandafter{\prevchapterdefs}% \toks6=\expandafter{\prevsectiondefs}% \toks8=\expandafter{\lastcolordefs}% \mark{% \the\toks0 \the\toks2 % 0: marks for @everyheadingmarks top \noexpand\or \the\toks4 \the\toks6 % 1: for @everyheadingmarks bottom \noexpand\else \the\toks8 % 2: color marks }% } % \gettopheadingmarks, \getbottomheadingmarks, % \getcolormarks - extract needed part of mark. % % \topmark doesn't work for the very first chapter (after the title % page or the contents), so we use \firstmark there -- this gets us % the mark with the chapter defs, unless the user sneaks in, e.g., % @setcolor (or @url, or @link, etc.) between @contents and the very % first @chapter. \def\gettopheadingmarks{% \ifcase0\topmark\fi \ifx\thischapter\empty \ifcase0\firstmark\fi \fi } \def\getbottomheadingmarks{\ifcase1\botmark\fi} \def\getcolormarks{\ifcase2\topmark\fi} % Avoid "undefined control sequence" errors. \def\lastchapterdefs{} \def\lastsectiondefs{} \def\lastsection{} \def\prevchapterdefs{} \def\prevsectiondefs{} \def\lastcolordefs{} % Margin to add to right of even pages, to left of odd pages. \newdimen\bindingoffset \newdimen\normaloffset \newdimen\txipagewidth \newdimen\txipageheight % Main output routine. % \chardef\PAGE = 255 \output = {\onepageout{\pagecontents\PAGE}} \newbox\headlinebox \newbox\footlinebox % \onepageout takes a vbox as an argument. % \shipout a vbox for a single page, adding an optional header, footer, % cropmarks, and footnote. This also causes index entries for this page % to be written to the auxiliary files. % \def\onepageout#1{% \ifcropmarks \hoffset=0pt \else \hoffset=\normaloffset \fi % \ifodd\pageno \advance\hoffset by \bindingoffset \else \advance\hoffset by -\bindingoffset\fi % % Common context changes for both heading and footing. % Do this outside of the \shipout so @code etc. will be expanded in % the headline as they should be, not taken literally (outputting ''code). \def\commmonheadfootline{\let\hsize=\txipagewidth \texinfochars} % % Retrieve the information for the headings from the marks in the page, % and call Plain TeX's \makeheadline and \makefootline, which use the % values in \headline and \footline. % % This is used to check if we are on the first page of a chapter. \ifcase1\topmark\fi \let\prevchaptername\thischaptername \ifcase0\firstmark\fi \let\curchaptername\thischaptername % \ifodd\pageno \getoddheadingmarks \else \getevenheadingmarks \fi \ifodd\pageno \getoddfootingmarks \else \getevenfootingmarks \fi % \ifx\curchaptername\prevchaptername \let\thischapterheading\thischapter \else % \thischapterheading is the same as \thischapter except it is blank % for the first page of a chapter. This is to prevent the chapter name % being shown twice. \def\thischapterheading{}% \fi % \global\setbox\headlinebox = \vbox{\commmonheadfootline \makeheadline}% \global\setbox\footlinebox = \vbox{\commmonheadfootline \makefootline}% % {% % Set context for writing to auxiliary files like index files. % Have to do this stuff outside the \shipout because we want it to % take effect in \write's, yet the group defined by the \vbox ends % before the \shipout runs. % \indexdummies % don't expand commands in the output. \normalturnoffactive % \ in index entries must not stay \, e.g., if % the page break happens to be in the middle of an example. % We don't want .vr (or whatever) entries like this: % \entry{{\indexbackslash }acronym}{32}{\code {\acronym}} % "\acronym" won't work when it's read back in; % it needs to be % {\code {{\backslashcurfont }acronym} \shipout\vbox{% % Do this early so pdf references go to the beginning of the page. \ifpdfmakepagedest \pdfdest name{\the\pageno} xyz\fi % \ifcropmarks \vbox to \outervsize\bgroup \hsize = \outerhsize \vskip-\topandbottommargin \vtop to0pt{% \line{\ewtop\hfil\ewtop}% \nointerlineskip \line{% \vbox{\moveleft\cornerthick\nstop}% \hfill \vbox{\moveright\cornerthick\nstop}% }% \vss}% \vskip\topandbottommargin \line\bgroup \hfil % center the page within the outer (page) hsize. \ifodd\pageno\hskip\bindingoffset\fi \vbox\bgroup \fi % \unvbox\headlinebox \pagebody{#1}% \ifdim\ht\footlinebox > 0pt % Only leave this space if the footline is nonempty. % (We lessened \vsize for it in \oddfootingyyy.) % The \baselineskip=24pt in plain's \makefootline has no effect. \vskip 24pt \unvbox\footlinebox \fi % \ifcropmarks \egroup % end of \vbox\bgroup \hfil\egroup % end of (centering) \line\bgroup \vskip\topandbottommargin plus1fill minus1fill \boxmaxdepth = \cornerthick \vbox to0pt{\vss \line{% \vbox{\moveleft\cornerthick\nsbot}% \hfill \vbox{\moveright\cornerthick\nsbot}% }% \nointerlineskip \line{\ewbot\hfil\ewbot}% }% \egroup % \vbox from first cropmarks clause \fi }% end of \shipout\vbox }% end of group with \indexdummies \advancepageno \ifnum\outputpenalty>-20000 \else\dosupereject\fi } \newinsert\margin \dimen\margin=\maxdimen % Main part of page, including any footnotes \def\pagebody#1{\vbox to\txipageheight{\boxmaxdepth=\maxdepth #1}} {\catcode`\@ =11 \gdef\pagecontents#1{\ifvoid\topins\else\unvbox\topins\fi % marginal hacks, juha@viisa.uucp (Juha Takala) \ifvoid\margin\else % marginal info is present \rlap{\kern\hsize\vbox to\z@{\kern1pt\box\margin \vss}}\fi \dimen@=\dp#1\relax \unvbox#1\relax \ifvoid\footins\else\vskip\skip\footins\footnoterule \unvbox\footins\fi \ifr@ggedbottom \kern-\dimen@ \vfil \fi} } % Here are the rules for the cropmarks. Note that they are % offset so that the space between them is truly \outerhsize or \outervsize % (P. A. MacKay, 12 November, 1986) % \def\ewtop{\vrule height\cornerthick depth0pt width\cornerlong} \def\nstop{\vbox {\hrule height\cornerthick depth\cornerlong width\cornerthick}} \def\ewbot{\vrule height0pt depth\cornerthick width\cornerlong} \def\nsbot{\vbox {\hrule height\cornerlong depth\cornerthick width\cornerthick}} % Argument parsing % Parse an argument, then pass it to #1. The argument is the rest of % the input line (except we remove a trailing comment). #1 should be a % macro which expects an ordinary undelimited TeX argument. % For example, \def\foo{\parsearg\fooxxx}. % \def\parsearg{\parseargusing{}} \def\parseargusing#1#2{% \def\argtorun{#2}% \begingroup \obeylines \spaceisspace #1% \parseargline\empty% Insert the \empty token, see \finishparsearg below. } {\obeylines % \gdef\parseargline#1^^M{% \endgroup % End of the group started in \parsearg. \argremovecomment #1\comment\ArgTerm% }% } % First remove any @comment, then any @c comment. Also remove a @texinfoc % comment (see \scanmacro for details). Pass the result on to \argcheckspaces. \def\argremovecomment#1\comment#2\ArgTerm{\argremovec #1\c\ArgTerm} \def\argremovec#1\c#2\ArgTerm{\argremovetexinfoc #1\texinfoc\ArgTerm} \def\argremovetexinfoc#1\texinfoc#2\ArgTerm{\argcheckspaces#1\^^M\ArgTerm} % Each occurrence of `\^^M' or `<space>\^^M' is replaced by a single space. % % \argremovec might leave us with trailing space, e.g., % @end itemize @c foo % This space token undergoes the same procedure and is eventually removed % by \finishparsearg. % \def\argcheckspaces#1\^^M{\argcheckspacesX#1\^^M \^^M} \def\argcheckspacesX#1 \^^M{\argcheckspacesY#1\^^M} \def\argcheckspacesY#1\^^M#2\^^M#3\ArgTerm{% \def\temp{#3}% \ifx\temp\empty % Do not use \next, perhaps the caller of \parsearg uses it; reuse \temp: \let\temp\finishparsearg \else \let\temp\argcheckspaces \fi % Put the space token in: \temp#1 #3\ArgTerm } % If a _delimited_ argument is enclosed in braces, they get stripped; so % to get _exactly_ the rest of the line, we had to prevent such situation. % We prepended an \empty token at the very beginning and we expand it now, % just before passing the control to \argtorun. % (Similarly, we have to think about #3 of \argcheckspacesY above: it is % either the null string, or it ends with \^^M---thus there is no danger % that a pair of braces would be stripped. % % But first, we have to remove the trailing space token. % \def\finishparsearg#1 \ArgTerm{\expandafter\argtorun\expandafter{#1}} % \parseargdef - define a command taking an argument on the line % % \parseargdef\foo{...} % is roughly equivalent to % \def\foo{\parsearg\Xfoo} % \def\Xfoo#1{...} \def\parseargdef#1{% \expandafter \doparseargdef \csname\string#1\endcsname #1% } \def\doparseargdef#1#2{% \def#2{\parsearg#1}% \def#1##1% } % Several utility definitions with active space: { \obeyspaces \gdef\obeyedspace{ } % Make each space character in the input produce a normal interword % space in the output. Don't allow a line break at this space, as this % is used only in environments like @example, where each line of input % should produce a line of output anyway. % \gdef\sepspaces{\obeyspaces\let =\tie} % If an index command is used in an @example environment, any spaces % therein should become regular spaces in the raw index file, not the % expansion of \tie (\leavevmode \penalty \@M \ ). \gdef\unsepspaces{\let =\space} } \def\flushcr{\ifx\par\lisppar \def\next##1{}\else \let\next=\relax \fi \next} % Define the framework for environments in texinfo.tex. It's used like this: % % \envdef\foo{...} % \def\Efoo{...} % % It's the responsibility of \envdef to insert \begingroup before the % actual body; @end closes the group after calling \Efoo. \envdef also % defines \thisenv, so the current environment is known; @end checks % whether the environment name matches. The \checkenv macro can also be % used to check whether the current environment is the one expected. % % Non-false conditionals (@iftex, @ifset) don't fit into this, so they % are not treated as environments; they don't open a group. (The % implementation of @end takes care not to call \endgroup in this % special case.) % At run-time, environments start with this: \def\startenvironment#1{\begingroup\def\thisenv{#1}} % initialize \let\thisenv\empty % ... but they get defined via ``\envdef\foo{...}'': \long\def\envdef#1#2{\def#1{\startenvironment#1#2}} \def\envparseargdef#1#2{\parseargdef#1{\startenvironment#1#2}} % Check whether we're in the right environment: \def\checkenv#1{% \def\temp{#1}% \ifx\thisenv\temp \else \badenverr \fi } % Environment mismatch, #1 expected: \def\badenverr{% \errhelp = \EMsimple \errmessage{This command can appear only \inenvironment\temp, not \inenvironment\thisenv}% } \def\inenvironment#1{% \ifx#1\empty outside of any environment% \else in environment \expandafter\string#1% \fi } % @end foo executes the definition of \Efoo. % But first, it executes a specialized version of \checkenv % \parseargdef\end{% \if 1\csname iscond.#1\endcsname \else % The general wording of \badenverr may not be ideal. \expandafter\checkenv\csname#1\endcsname \csname E#1\endcsname \endgroup \fi } \newhelp\EMsimple{Press RETURN to continue.} % Be sure we're in horizontal mode when doing a tie, since we make space % equivalent to this in @example-like environments. Otherwise, a space % at the beginning of a line will start with \penalty -- and % since \penalty is valid in vertical mode, we'd end up putting the % penalty on the vertical list instead of in the new paragraph. {\catcode`@ = 11 % Avoid using \@M directly, because that causes trouble % if the definition is written into an index file. \global\let\tiepenalty = \@M \gdef\tie{\leavevmode\penalty\tiepenalty\ } } % @: forces normal size whitespace following. \def\:{\spacefactor=1000 } % @* forces a line break. \def\*{\unskip\hfil\break\hbox{}\ignorespaces} % @/ allows a line break. \let\/=\allowbreak % @. is an end-of-sentence period. \def\.{.\spacefactor=\endofsentencespacefactor\space} % @! is an end-of-sentence bang. \def\!{!\spacefactor=\endofsentencespacefactor\space} % @? is an end-of-sentence query. \def\?{?\spacefactor=\endofsentencespacefactor\space} % @frenchspacing on|off says whether to put extra space after punctuation. % \def\onword{on} \def\offword{off} % \parseargdef\frenchspacing{% \def\temp{#1}% \ifx\temp\onword \plainfrenchspacing \else\ifx\temp\offword \plainnonfrenchspacing \else \errhelp = \EMsimple \errmessage{Unknown @frenchspacing option `\temp', must be on|off}% \fi\fi } % @w prevents a word break. Without the \leavevmode, @w at the % beginning of a paragraph, when TeX is still in vertical mode, would % produce a whole line of output instead of starting the paragraph. \def\w#1{\leavevmode\hbox{#1}} % @group ... @end group forces ... to be all on one page, by enclosing % it in a TeX vbox. We use \vtop instead of \vbox to construct the box % to keep its height that of a normal line. According to the rules for % \topskip (p.114 of the TeXbook), the glue inserted is % max (\topskip - \ht (first item), 0). If that height is large, % therefore, no glue is inserted, and the space between the headline and % the text is small, which looks bad. % % Another complication is that the group might be very large. This can % cause the glue on the previous page to be unduly stretched, because it % does not have much material. In this case, it's better to add an % explicit \vfill so that the extra space is at the bottom. The % threshold for doing this is if the group is more than \vfilllimit % percent of a page (\vfilllimit can be changed inside of @tex). % \newbox\groupbox \def\vfilllimit{0.7} % \envdef\group{% \ifnum\catcode`\^^M=\active \else \errhelp = \groupinvalidhelp \errmessage{@group invalid in context where filling is enabled}% \fi \startsavinginserts % \setbox\groupbox = \vtop\bgroup % Do @comment since we are called inside an environment such as % @example, where each end-of-line in the input causes an % end-of-line in the output. We don't want the end-of-line after % the `@group' to put extra space in the output. Since @group % should appear on a line by itself (according to the Texinfo % manual), we don't worry about eating any user text. \comment } % % The \vtop produces a box with normal height and large depth; thus, TeX puts % \baselineskip glue before it, and (when the next line of text is done) % \lineskip glue after it. Thus, space below is not quite equal to space % above. But it's pretty close. \def\Egroup{% % To get correct interline space between the last line of the group % and the first line afterwards, we have to propagate \prevdepth. \endgraf % Not \par, as it may have been set to \lisppar. \global\dimen1 = \prevdepth \egroup % End the \vtop. \addgroupbox \prevdepth = \dimen1 \checkinserts } \def\addgroupbox{ % \dimen0 is the vertical size of the group's box. \dimen0 = \ht\groupbox \advance\dimen0 by \dp\groupbox % \dimen2 is how much space is left on the page (more or less). \dimen2 = \txipageheight \advance\dimen2 by -\pagetotal % if the group doesn't fit on the current page, and it's a big big % group, force a page break. \ifdim \dimen0 > \dimen2 \ifdim \pagetotal < \vfilllimit\txipageheight \page \fi \fi \box\groupbox } % % TeX puts in an \escapechar (i.e., `@') at the beginning of the help % message, so this ends up printing `@group can only ...'. % \newhelp\groupinvalidhelp{% group can only be used in environments such as @example,^^J% where each line of input produces a line of output.} % @need space-in-mils % forces a page break if there is not space-in-mils remaining. \newdimen\mil \mil=0.001in \parseargdef\need{% % Ensure vertical mode, so we don't make a big box in the middle of a % paragraph. \par % % If the @need value is less than one line space, it's useless. \dimen0 = #1\mil \dimen2 = \ht\strutbox \advance\dimen2 by \dp\strutbox \ifdim\dimen0 > \dimen2 % % Do a \strut just to make the height of this box be normal, so the % normal leading is inserted relative to the preceding line. % And a page break here is fine. \vtop to #1\mil{\strut\vfil}% % % TeX does not even consider page breaks if a penalty added to the % main vertical list is 10000 or more. But in order to see if the % empty box we just added fits on the page, we must make it consider % page breaks. On the other hand, we don't want to actually break the % page after the empty box. So we use a penalty of 9999. % % There is an extremely small chance that TeX will actually break the % page at this \penalty, if there are no other feasible breakpoints in % sight. (If the user is using lots of big @group commands, which % almost-but-not-quite fill up a page, TeX will have a hard time doing % good page breaking, for example.) However, I could not construct an % example where a page broke at this \penalty; if it happens in a real % document, then we can reconsider our strategy. \penalty9999 % % Back up by the size of the box, whether we did a page break or not. \kern -#1\mil % % Do not allow a page break right after this kern. \nobreak \fi } % @br forces paragraph break (and is undocumented). \let\br = \par % @page forces the start of a new page. % \def\page{\par\vfill\supereject} % @exdent text.... % outputs text on separate line in roman font, starting at standard page margin % This records the amount of indent in the innermost environment. % That's how much \exdent should take out. \newskip\exdentamount % This defn is used inside fill environments such as @defun. \parseargdef\exdent{\hfil\break\hbox{\kern -\exdentamount{\rm#1}}\hfil\break} % This defn is used inside nofill environments such as @example. \parseargdef\nofillexdent{{\advance \leftskip by -\exdentamount \leftline{\hskip\leftskip{\rm#1}}}} % @inmargin{WHICH}{TEXT} puts TEXT in the WHICH margin next to the current % paragraph. For more general purposes, use the \margin insertion % class. WHICH is `l' or `r'. Not documented, written for gawk manual. % \newskip\inmarginspacing \inmarginspacing=1cm \def\strutdepth{\dp\strutbox} % \def\doinmargin#1#2{\strut\vadjust{% \nobreak \kern-\strutdepth \vtop to \strutdepth{% \baselineskip=\strutdepth \vss % if you have multiple lines of stuff to put here, you'll need to % make the vbox yourself of the appropriate size. \ifx#1l% \llap{\ignorespaces #2\hskip\inmarginspacing}% \else \rlap{\hskip\hsize \hskip\inmarginspacing \ignorespaces #2}% \fi \null }% }} \def\inleftmargin{\doinmargin l} \def\inrightmargin{\doinmargin r} % % @inmargin{TEXT [, RIGHT-TEXT]} % (if RIGHT-TEXT is given, use TEXT for left page, RIGHT-TEXT for right; % else use TEXT for both). % \def\inmargin#1{\parseinmargin #1,,\finish} \def\parseinmargin#1,#2,#3\finish{% not perfect, but better than nothing. \setbox0 = \hbox{\ignorespaces #2}% \ifdim\wd0 > 0pt \def\lefttext{#1}% have both texts \def\righttext{#2}% \else \def\lefttext{#1}% have only one text \def\righttext{#1}% \fi % \ifodd\pageno \def\temp{\inrightmargin\righttext}% odd page -> outside is right margin \else \def\temp{\inleftmargin\lefttext}% \fi \temp } % @include FILE -- \input text of FILE. % \def\include{\parseargusing\filenamecatcodes\includezzz} \def\includezzz#1{% \pushthisfilestack \def\thisfile{#1}% {% \makevalueexpandable % we want to expand any @value in FILE. \turnoffactive % and allow special characters in the expansion \indexnofonts % Allow `@@' and other weird things in file names. \wlog{texinfo.tex: doing @include of #1^^J}% \edef\temp{\noexpand\input #1 }% % % This trickery is to read FILE outside of a group, in case it makes % definitions, etc. \expandafter }\temp \popthisfilestack } \def\filenamecatcodes{% \catcode`\\=\other \catcode`~=\other \catcode`^=\other \catcode`_=\other \catcode`|=\other \catcode`<=\other \catcode`>=\other \catcode`+=\other \catcode`-=\other \catcode`\`=\other \catcode`\'=\other } \def\pushthisfilestack{% \expandafter\pushthisfilestackX\popthisfilestack\StackTerm } \def\pushthisfilestackX{% \expandafter\pushthisfilestackY\thisfile\StackTerm } \def\pushthisfilestackY #1\StackTerm #2\StackTerm {% \gdef\popthisfilestack{\gdef\thisfile{#1}\gdef\popthisfilestack{#2}}% } \def\popthisfilestack{\errthisfilestackempty} \def\errthisfilestackempty{\errmessage{Internal error: the stack of filenames is empty.}} % \def\thisfile{} % @center line % outputs that line, centered. % \parseargdef\center{% \ifhmode \let\centersub\centerH \else \let\centersub\centerV \fi \centersub{\hfil \ignorespaces#1\unskip \hfil}% \let\centersub\relax % don't let the definition persist, just in case } \def\centerH#1{{% \hfil\break \advance\hsize by -\leftskip \advance\hsize by -\rightskip \line{#1}% \break }} % \newcount\centerpenalty \def\centerV#1{% % The idea here is the same as in \startdefun, \cartouche, etc.: if % @center is the first thing after a section heading, we need to wipe % out the negative parskip inserted by \sectionheading, but still % prevent a page break here. \centerpenalty = \lastpenalty \ifnum\centerpenalty>10000 \vskip\parskip \fi \ifnum\centerpenalty>9999 \penalty\centerpenalty \fi \line{\kern\leftskip #1\kern\rightskip}% } % @sp n outputs n lines of vertical space % \parseargdef\sp{\vskip #1\baselineskip} % @comment ...line which is ignored... % @c is the same as @comment % @ignore ... @end ignore is another way to write a comment % \def\comment{\begingroup \catcode`\^^M=\active% \catcode`\@=\other \catcode`\{=\other \catcode`\}=\other\commentxxx}% {\catcode`\^^M=\active% \gdef\commentxxx#1^^M{\endgroup% \futurelet\nexttoken\commentxxxx}% \gdef\commentxxxx{\ifx\nexttoken\aftermacro\expandafter\comment\fi}% } \def\c{\begingroup \catcode`\^^M=\active% \catcode`\@=\other \catcode`\{=\other \catcode`\}=\other% \cxxx} {\catcode`\^^M=\active \gdef\cxxx#1^^M{\endgroup}} % See comment in \scanmacro about why the definitions of @c and @comment differ % @paragraphindent NCHARS % We'll use ems for NCHARS, close enough. % NCHARS can also be the word `asis' or `none'. % We cannot feasibly implement @paragraphindent asis, though. % \def\asisword{asis} % no translation, these are keywords \def\noneword{none} % \parseargdef\paragraphindent{% \def\temp{#1}% \ifx\temp\asisword \else \ifx\temp\noneword \defaultparindent = 0pt \else \defaultparindent = #1em \fi \fi \parindent = \defaultparindent } % @exampleindent NCHARS % We'll use ems for NCHARS like @paragraphindent. % It seems @exampleindent asis isn't necessary, but % I preserve it to make it similar to @paragraphindent. \parseargdef\exampleindent{% \def\temp{#1}% \ifx\temp\asisword \else \ifx\temp\noneword \lispnarrowing = 0pt \else \lispnarrowing = #1em \fi \fi } % @firstparagraphindent WORD % If WORD is `none', then suppress indentation of the first paragraph % after a section heading. If WORD is `insert', then do indent at such % paragraphs. % % The paragraph indentation is suppressed or not by calling % \suppressfirstparagraphindent, which the sectioning commands do. % We switch the definition of this back and forth according to WORD. % By default, we suppress indentation. % \def\suppressfirstparagraphindent{\dosuppressfirstparagraphindent} \def\insertword{insert} % \parseargdef\firstparagraphindent{% \def\temp{#1}% \ifx\temp\noneword \let\suppressfirstparagraphindent = \dosuppressfirstparagraphindent \else\ifx\temp\insertword \let\suppressfirstparagraphindent = \relax \else \errhelp = \EMsimple \errmessage{Unknown @firstparagraphindent option `\temp'}% \fi\fi } % Here is how we actually suppress indentation. Redefine \everypar to % \kern backwards by \parindent, and then reset itself to empty. % % We also make \indent itself not actually do anything until the next % paragraph. % \gdef\dosuppressfirstparagraphindent{% \gdef\indent {\restorefirstparagraphindent \indent}% \gdef\noindent{\restorefirstparagraphindent \noindent}% \global\everypar = {\kern -\parindent \restorefirstparagraphindent}% } % \gdef\restorefirstparagraphindent{% \global\let\indent = \ptexindent \global\let\noindent = \ptexnoindent \global\everypar = {}% } % @refill is a no-op. \let\refill=\relax % @setfilename INFO-FILENAME - ignored \let\setfilename=\comment % @bye. \outer\def\bye{\pagealignmacro\tracingstats=1\ptexend} \message{pdf,} % adobe `portable' document format \newcount\tempnum \newcount\lnkcount \newtoks\filename \newcount\filenamelength \newcount\pgn \newtoks\toksA \newtoks\toksB \newtoks\toksC \newtoks\toksD \newbox\boxA \newbox\boxB \newcount\countA \newif\ifpdf \newif\ifpdfmakepagedest % % For LuaTeX % \newif\iftxiuseunicodedestname \txiuseunicodedestnamefalse % For pdfTeX etc. \ifx\luatexversion\thisisundefined \else % Use Unicode destination names \txiuseunicodedestnametrue % Escape PDF strings with converting UTF-16 from UTF-8 \begingroup \catcode`\%=12 \directlua{ function UTF16oct(str) tex.sprint(string.char(0x5c) .. '376' .. string.char(0x5c) .. '377') for c in string.utfvalues(str) do if c < 0x10000 then tex.sprint( string.format(string.char(0x5c) .. string.char(0x25) .. '03o' .. string.char(0x5c) .. string.char(0x25) .. '03o', (c / 256), (c % 256))) else c = c - 0x10000 local c_hi = c / 1024 + 0xd800 local c_lo = c % 1024 + 0xdc00 tex.sprint( string.format(string.char(0x5c) .. string.char(0x25) .. '03o' .. string.char(0x5c) .. string.char(0x25) .. '03o' .. string.char(0x5c) .. string.char(0x25) .. '03o' .. string.char(0x5c) .. string.char(0x25) .. '03o', (c_hi / 256), (c_hi % 256), (c_lo / 256), (c_lo % 256))) end end end } \endgroup \def\pdfescapestrutfsixteen#1{\directlua{UTF16oct('\luaescapestring{#1}')}} % Escape PDF strings without converting \begingroup \directlua{ function PDFescstr(str) for c in string.bytes(str) do if c <= 0x20 or c >= 0x80 or c == 0x28 or c == 0x29 or c == 0x5c then tex.sprint( string.format(string.char(0x5c) .. string.char(0x25) .. '03o', c)) else tex.sprint(string.char(c)) end end end } \endgroup \def\pdfescapestring#1{\directlua{PDFescstr('\luaescapestring{#1}')}} \ifnum\luatexversion>84 % For LuaTeX >= 0.85 \def\pdfdest{\pdfextension dest} \let\pdfoutput\outputmode \def\pdfliteral{\pdfextension literal} \def\pdfcatalog{\pdfextension catalog} \def\pdftexversion{\numexpr\pdffeedback version\relax} \let\pdfximage\saveimageresource \let\pdfrefximage\useimageresource \let\pdflastximage\lastsavedimageresourceindex \def\pdfendlink{\pdfextension endlink\relax} \def\pdfoutline{\pdfextension outline} \def\pdfstartlink{\pdfextension startlink} \def\pdffontattr{\pdfextension fontattr} \def\pdfobj{\pdfextension obj} \def\pdflastobj{\numexpr\pdffeedback lastobj\relax} \let\pdfpagewidth\pagewidth \let\pdfpageheight\pageheight \edef\pdfhorigin{\pdfvariable horigin} \edef\pdfvorigin{\pdfvariable vorigin} \fi \fi % when pdftex is run in dvi mode, \pdfoutput is defined (so \pdfoutput=1 % can be set). So we test for \relax and 0 as well as being undefined. \ifx\pdfoutput\thisisundefined \else \ifx\pdfoutput\relax \else \ifcase\pdfoutput \else \pdftrue \fi \fi \fi % PDF uses PostScript string constants for the names of xref targets, % for display in the outlines, and in other places. Thus, we have to % double any backslashes. Otherwise, a name like "\node" will be % interpreted as a newline (\n), followed by o, d, e. Not good. % % See http://www.ntg.nl/pipermail/ntg-pdftex/2004-July/000654.html and % related messages. The final outcome is that it is up to the TeX user % to double the backslashes and otherwise make the string valid, so % that's what we do. pdftex 1.30.0 (ca.2005) introduced a primitive to % do this reliably, so we use it. % #1 is a control sequence in which to do the replacements, % which we \xdef. \def\txiescapepdf#1{% \ifx\pdfescapestring\thisisundefined % No primitive available; should we give a warning or log? % Many times it won't matter. \xdef#1{#1}% \else % The expandable \pdfescapestring primitive escapes parentheses, % backslashes, and other special chars. \xdef#1{\pdfescapestring{#1}}% \fi } \def\txiescapepdfutfsixteen#1{% \ifx\pdfescapestrutfsixteen\thisisundefined % No UTF-16 converting macro available. \txiescapepdf{#1}% \else \xdef#1{\pdfescapestrutfsixteen{#1}}% \fi } \newhelp\nopdfimagehelp{Texinfo supports .png, .jpg, .jpeg, and .pdf images with PDF output, and none of those formats could be found. (.eps cannot be supported due to the design of the PDF format; use regular TeX (DVI output) for that.)} \ifpdf % % Color manipulation macros using ideas from pdfcolor.tex, % except using rgb instead of cmyk; the latter is said to render as a % very dark gray on-screen and a very dark halftone in print, instead % of actual black. The dark red here is dark enough to print on paper as % nearly black, but still distinguishable for online viewing. We use % black by default, though. \def\rgbDarkRed{0.50 0.09 0.12} \def\rgbBlack{0 0 0} % % rg sets the color for filling (usual text, etc.); % RG sets the color for stroking (thin rules, e.g., normal _'s). \def\pdfsetcolor#1{\pdfliteral{#1 rg #1 RG}} % % Set color, and create a mark which defines \thiscolor accordingly, % so that \makeheadline knows which color to restore. \def\setcolor#1{% \xdef\lastcolordefs{\gdef\noexpand\thiscolor{#1}}% \domark \pdfsetcolor{#1}% } % \def\maincolor{\rgbBlack} \pdfsetcolor{\maincolor} \edef\thiscolor{\maincolor} \def\lastcolordefs{} % \def\makefootline{% \baselineskip24pt \line{\pdfsetcolor{\maincolor}\the\footline}% } % \def\makeheadline{% \vbox to 0pt{% \vskip-22.5pt \line{% \vbox to8.5pt{}% % Extract \thiscolor definition from the marks. \getcolormarks % Typeset the headline with \maincolor, then restore the color. \pdfsetcolor{\maincolor}\the\headline\pdfsetcolor{\thiscolor}% }% \vss }% \nointerlineskip } % % \pdfcatalog{/PageMode /UseOutlines} % % #1 is image name, #2 width (might be empty/whitespace), #3 height (ditto). \def\dopdfimage#1#2#3{% \def\pdfimagewidth{#2}\setbox0 = \hbox{\ignorespaces #2}% \def\pdfimageheight{#3}\setbox2 = \hbox{\ignorespaces #3}% % % pdftex (and the PDF format) support .pdf, .png, .jpg (among % others). Let's try in that order, PDF first since if % someone has a scalable image, presumably better to use that than a % bitmap. \let\pdfimgext=\empty \begingroup \openin 1 #1.pdf \ifeof 1 \openin 1 #1.PDF \ifeof 1 \openin 1 #1.png \ifeof 1 \openin 1 #1.jpg \ifeof 1 \openin 1 #1.jpeg \ifeof 1 \openin 1 #1.JPG \ifeof 1 \errhelp = \nopdfimagehelp \errmessage{Could not find image file #1 for pdf}% \else \gdef\pdfimgext{JPG}% \fi \else \gdef\pdfimgext{jpeg}% \fi \else \gdef\pdfimgext{jpg}% \fi \else \gdef\pdfimgext{png}% \fi \else \gdef\pdfimgext{PDF}% \fi \else \gdef\pdfimgext{pdf}% \fi \closein 1 \endgroup % % without \immediate, ancient pdftex seg faults when the same image is % included twice. (Version 3.14159-pre-1.0-unofficial-20010704.) \ifnum\pdftexversion < 14 \immediate\pdfimage \else \immediate\pdfximage \fi \ifdim \wd0 >0pt width \pdfimagewidth \fi \ifdim \wd2 >0pt height \pdfimageheight \fi \ifnum\pdftexversion<13 #1.\pdfimgext \else {#1.\pdfimgext}% \fi \ifnum\pdftexversion < 14 \else \pdfrefximage \pdflastximage \fi} % \def\setpdfdestname#1{{% % We have to set dummies so commands such as @code, and characters % such as \, aren't expanded when present in a section title. \indexnofonts \makevalueexpandable \turnoffactive \iftxiuseunicodedestname \ifx \declaredencoding \latone % Pass through Latin-1 characters. % LuaTeX with byte wise I/O converts Latin-1 characters to Unicode. \else \ifx \declaredencoding \utfeight % Pass through Unicode characters. \else % Use ASCII approximations in destination names. \passthroughcharsfalse \fi \fi \else % Use ASCII approximations in destination names. \passthroughcharsfalse \fi \def\pdfdestname{#1}% \txiescapepdf\pdfdestname }} % \def\setpdfoutlinetext#1{{% \indexnofonts \makevalueexpandable \turnoffactive \ifx \declaredencoding \latone % The PDF format can use an extended form of Latin-1 in bookmark % strings. See Appendix D of the PDF Reference, Sixth Edition, for % the "PDFDocEncoding". \passthroughcharstrue % Pass through Latin-1 characters. % LuaTeX: Convert to Unicode % pdfTeX: Use Latin-1 as PDFDocEncoding \def\pdfoutlinetext{#1}% \else \ifx \declaredencoding \utfeight \ifx\luatexversion\thisisundefined % For pdfTeX with UTF-8. % TODO: the PDF format can use UTF-16 in bookmark strings, % but the code for this isn't done yet. % Use ASCII approximations. \passthroughcharsfalse \def\pdfoutlinetext{#1}% \else % For LuaTeX with UTF-8. % Pass through Unicode characters for title texts. \passthroughcharstrue \def\pdfoutlinetext{#1}% \fi \else % For non-Latin-1 or non-UTF-8 encodings. % Use ASCII approximations. \passthroughcharsfalse \def\pdfoutlinetext{#1}% \fi \fi % LuaTeX: Convert to UTF-16 % pdfTeX: Use Latin-1 as PDFDocEncoding \txiescapepdfutfsixteen\pdfoutlinetext }} % \def\pdfmkdest#1{% \setpdfdestname{#1}% \safewhatsit{\pdfdest name{\pdfdestname} xyz}% } % % used to mark target names; must be expandable. \def\pdfmkpgn#1{#1} % % by default, use black for everything. \def\urlcolor{\rgbBlack} \def\linkcolor{\rgbBlack} \def\endlink{\setcolor{\maincolor}\pdfendlink} % % Adding outlines to PDF; macros for calculating structure of outlines % come from Petr Olsak \def\expnumber#1{\expandafter\ifx\csname#1\endcsname\relax 0% \else \csname#1\endcsname \fi} \def\advancenumber#1{\tempnum=\expnumber{#1}\relax \advance\tempnum by 1 \expandafter\xdef\csname#1\endcsname{\the\tempnum}} % % #1 is the section text, which is what will be displayed in the % outline by the pdf viewer. #2 is the pdf expression for the number % of subentries (or empty, for subsubsections). #3 is the node text, % which might be empty if this toc entry had no corresponding node. % #4 is the page number % \def\dopdfoutline#1#2#3#4{% % Generate a link to the node text if that exists; else, use the % page number. We could generate a destination for the section % text in the case where a section has no node, but it doesn't % seem worth the trouble, since most documents are normally structured. \setpdfoutlinetext{#1} \setpdfdestname{#3} \ifx\pdfdestname\empty \def\pdfdestname{#4}% \fi % \pdfoutline goto name{\pdfmkpgn{\pdfdestname}}#2{\pdfoutlinetext}% } % \def\pdfmakeoutlines{% \begingroup % Read toc silently, to get counts of subentries for \pdfoutline. \def\partentry##1##2##3##4{}% ignore parts in the outlines \def\numchapentry##1##2##3##4{% \def\thischapnum{##2}% \def\thissecnum{0}% \def\thissubsecnum{0}% }% \def\numsecentry##1##2##3##4{% \advancenumber{chap\thischapnum}% \def\thissecnum{##2}% \def\thissubsecnum{0}% }% \def\numsubsecentry##1##2##3##4{% \advancenumber{sec\thissecnum}% \def\thissubsecnum{##2}% }% \def\numsubsubsecentry##1##2##3##4{% \advancenumber{subsec\thissubsecnum}% }% \def\thischapnum{0}% \def\thissecnum{0}% \def\thissubsecnum{0}% % % use \def rather than \let here because we redefine \chapentry et % al. a second time, below. \def\appentry{\numchapentry}% \def\appsecentry{\numsecentry}% \def\appsubsecentry{\numsubsecentry}% \def\appsubsubsecentry{\numsubsubsecentry}% \def\unnchapentry{\numchapentry}% \def\unnsecentry{\numsecentry}% \def\unnsubsecentry{\numsubsecentry}% \def\unnsubsubsecentry{\numsubsubsecentry}% \readdatafile{toc}% % % Read toc second time, this time actually producing the outlines. % The `-' means take the \expnumber as the absolute number of % subentries, which we calculated on our first read of the .toc above. % % We use the node names as the destinations. \def\numchapentry##1##2##3##4{% \dopdfoutline{##1}{count-\expnumber{chap##2}}{##3}{##4}}% \def\numsecentry##1##2##3##4{% \dopdfoutline{##1}{count-\expnumber{sec##2}}{##3}{##4}}% \def\numsubsecentry##1##2##3##4{% \dopdfoutline{##1}{count-\expnumber{subsec##2}}{##3}{##4}}% \def\numsubsubsecentry##1##2##3##4{% count is always zero \dopdfoutline{##1}{}{##3}{##4}}% % % PDF outlines are displayed using system fonts, instead of % document fonts. Therefore we cannot use special characters, % since the encoding is unknown. For example, the eogonek from % Latin 2 (0xea) gets translated to a | character. Info from % Staszek Wawrykiewicz, 19 Jan 2004 04:09:24 +0100. % % TODO this right, we have to translate 8-bit characters to % their "best" equivalent, based on the @documentencoding. Too % much work for too little return. Just use the ASCII equivalents % we use for the index sort strings. % \indexnofonts \setupdatafile % We can have normal brace characters in the PDF outlines, unlike % Texinfo index files. So set that up. \def\{{\lbracecharliteral}% \def\}{\rbracecharliteral}% \catcode`\\=\active \otherbackslash \input \tocreadfilename \endgroup } {\catcode`[=1 \catcode`]=2 \catcode`{=\other \catcode`}=\other \gdef\lbracecharliteral[{]% \gdef\rbracecharliteral[}]% ] % \def\skipspaces#1{\def\PP{#1}\def\D{|}% \ifx\PP\D\let\nextsp\relax \else\let\nextsp\skipspaces \addtokens{\filename}{\PP}% \advance\filenamelength by 1 \fi \nextsp} \def\getfilename#1{% \filenamelength=0 % If we don't expand the argument now, \skipspaces will get % snagged on things like "@value{foo}". \edef\temp{#1}% \expandafter\skipspaces\temp|\relax } \ifnum\pdftexversion < 14 \let \startlink \pdfannotlink \else \let \startlink \pdfstartlink \fi % make a live url in pdf output. \def\pdfurl#1{% \begingroup % it seems we really need yet another set of dummies; have not % tried to figure out what each command should do in the context % of @url. for now, just make @/ a no-op, that's the only one % people have actually reported a problem with. % \normalturnoffactive \def\@{@}% \let\/=\empty \makevalueexpandable % do we want to go so far as to use \indexnofonts instead of just % special-casing \var here? \def\var##1{##1}% % \leavevmode\setcolor{\urlcolor}% \startlink attr{/Border [0 0 0]}% user{/Subtype /Link /A << /S /URI /URI (#1) >>}% \endgroup} \def\pdfgettoks#1.{\setbox\boxA=\hbox{\toksA={#1.}\toksB={}\maketoks}} \def\addtokens#1#2{\edef\addtoks{\noexpand#1={\the#1#2}}\addtoks} \def\adn#1{\addtokens{\toksC}{#1}\global\countA=1\let\next=\maketoks} \def\poptoks#1#2|ENDTOKS|{\let\first=#1\toksD={#1}\toksA={#2}} \def\maketoks{% \expandafter\poptoks\the\toksA|ENDTOKS|\relax \ifx\first0\adn0 \else\ifx\first1\adn1 \else\ifx\first2\adn2 \else\ifx\first3\adn3 \else\ifx\first4\adn4 \else\ifx\first5\adn5 \else\ifx\first6\adn6 \else\ifx\first7\adn7 \else\ifx\first8\adn8 \else\ifx\first9\adn9 \else \ifnum0=\countA\else\makelink\fi \ifx\first.\let\next=\done\else \let\next=\maketoks \addtokens{\toksB}{\the\toksD} \ifx\first,\addtokens{\toksB}{\space}\fi \fi \fi\fi\fi\fi\fi\fi\fi\fi\fi\fi \next} \def\makelink{\addtokens{\toksB}% {\noexpand\pdflink{\the\toksC}}\toksC={}\global\countA=0} \def\pdflink#1{% \startlink attr{/Border [0 0 0]} goto name{\pdfmkpgn{#1}} \setcolor{\linkcolor}#1\endlink} \def\done{\edef\st{\global\noexpand\toksA={\the\toksB}}\st} \else % non-pdf mode \let\pdfmkdest = \gobble \let\pdfurl = \gobble \let\endlink = \relax \let\setcolor = \gobble \let\pdfsetcolor = \gobble \let\pdfmakeoutlines = \relax \fi % \ifx\pdfoutput % % For XeTeX % \ifx\XeTeXrevision\thisisundefined \else % % XeTeX version check % \ifnum\strcmp{\the\XeTeXversion\XeTeXrevision}{0.99996}>-1 % TeX Live 2016 contains XeTeX 0.99996 and xdvipdfmx 20160307. % It can use the `dvipdfmx:config' special (from TeX Live SVN r40941). % For avoiding PDF destination name replacement, we use this special % instead of xdvipdfmx's command line option `-C 0x0010'. \special{dvipdfmx:config C 0x0010} % XeTeX 0.99995+ comes with xdvipdfmx 20160307+. % It can handle Unicode destination names for PDF. \txiuseunicodedestnametrue \else % XeTeX < 0.99996 (TeX Live < 2016) cannot use the % `dvipdfmx:config' special. % So for avoiding PDF destination name replacement, % xdvipdfmx's command line option `-C 0x0010' is necessary. % % XeTeX < 0.99995 can not handle Unicode destination names for PDF % because xdvipdfmx 20150315 has a UTF-16 conversion issue. % It is fixed by xdvipdfmx 20160106 (TeX Live SVN r39753). \txiuseunicodedestnamefalse \fi % % Color support % \def\rgbDarkRed{0.50 0.09 0.12} \def\rgbBlack{0 0 0} % \def\pdfsetcolor#1{\special{pdf:scolor [#1]}} % % Set color, and create a mark which defines \thiscolor accordingly, % so that \makeheadline knows which color to restore. \def\setcolor#1{% \xdef\lastcolordefs{\gdef\noexpand\thiscolor{#1}}% \domark \pdfsetcolor{#1}% } % \def\maincolor{\rgbBlack} \pdfsetcolor{\maincolor} \edef\thiscolor{\maincolor} \def\lastcolordefs{} % \def\makefootline{% \baselineskip24pt \line{\pdfsetcolor{\maincolor}\the\footline}% } % \def\makeheadline{% \vbox to 0pt{% \vskip-22.5pt \line{% \vbox to8.5pt{}% % Extract \thiscolor definition from the marks. \getcolormarks % Typeset the headline with \maincolor, then restore the color. \pdfsetcolor{\maincolor}\the\headline\pdfsetcolor{\thiscolor}% }% \vss }% \nointerlineskip } % % PDF outline support % % Emulate pdfTeX primitive \def\pdfdest name#1 xyz{% \special{pdf:dest (#1) [@thispage /XYZ @xpos @ypos null]}% } % \def\setpdfdestname#1{{% % We have to set dummies so commands such as @code, and characters % such as \, aren't expanded when present in a section title. \indexnofonts \makevalueexpandable \turnoffactive \iftxiuseunicodedestname % Pass through Unicode characters. \else % Use ASCII approximations in destination names. \passthroughcharsfalse \fi \def\pdfdestname{#1}% \txiescapepdf\pdfdestname }} % \def\setpdfoutlinetext#1{{% \turnoffactive % Always use Unicode characters in title texts. \def\pdfoutlinetext{#1}% % For XeTeX, xdvipdfmx converts to UTF-16. % So we do not convert. \txiescapepdf\pdfoutlinetext }} % \def\pdfmkdest#1{% \setpdfdestname{#1}% \safewhatsit{\pdfdest name{\pdfdestname} xyz}% } % % by default, use black for everything. \def\urlcolor{\rgbBlack} \def\linkcolor{\rgbBlack} \def\endlink{\setcolor{\maincolor}\pdfendlink} % \def\dopdfoutline#1#2#3#4{% \setpdfoutlinetext{#1} \setpdfdestname{#3} \ifx\pdfdestname\empty \def\pdfdestname{#4}% \fi % \special{pdf:out [-] #2 << /Title (\pdfoutlinetext) /A << /S /GoTo /D (\pdfdestname) >> >> }% } % \def\pdfmakeoutlines{% \begingroup % % For XeTeX, counts of subentries are not necessary. % Therefore, we read toc only once. % % We use node names as destinations. \def\partentry##1##2##3##4{}% ignore parts in the outlines \def\numchapentry##1##2##3##4{% \dopdfoutline{##1}{1}{##3}{##4}}% \def\numsecentry##1##2##3##4{% \dopdfoutline{##1}{2}{##3}{##4}}% \def\numsubsecentry##1##2##3##4{% \dopdfoutline{##1}{3}{##3}{##4}}% \def\numsubsubsecentry##1##2##3##4{% \dopdfoutline{##1}{4}{##3}{##4}}% % \let\appentry\numchapentry% \let\appsecentry\numsecentry% \let\appsubsecentry\numsubsecentry% \let\appsubsubsecentry\numsubsubsecentry% \let\unnchapentry\numchapentry% \let\unnsecentry\numsecentry% \let\unnsubsecentry\numsubsecentry% \let\unnsubsubsecentry\numsubsubsecentry% % % For XeTeX, xdvipdfmx converts strings to UTF-16. % Therefore, the encoding and the language may not be considered. % \indexnofonts \setupdatafile % We can have normal brace characters in the PDF outlines, unlike % Texinfo index files. So set that up. \def\{{\lbracecharliteral}% \def\}{\rbracecharliteral}% \catcode`\\=\active \otherbackslash \input \tocreadfilename \endgroup } {\catcode`[=1 \catcode`]=2 \catcode`{=\other \catcode`}=\other \gdef\lbracecharliteral[{]% \gdef\rbracecharliteral[}]% ] \special{pdf:docview << /PageMode /UseOutlines >> } % ``\special{pdf:tounicode ...}'' is not necessary % because xdvipdfmx converts strings from UTF-8 to UTF-16 without it. % However, due to a UTF-16 conversion issue of xdvipdfmx 20150315, % ``\special{pdf:dest ...}'' cannot handle non-ASCII strings. % It is fixed by xdvipdfmx 20160106 (TeX Live SVN r39753). % \def\skipspaces#1{\def\PP{#1}\def\D{|}% \ifx\PP\D\let\nextsp\relax \else\let\nextsp\skipspaces \addtokens{\filename}{\PP}% \advance\filenamelength by 1 \fi \nextsp} \def\getfilename#1{% \filenamelength=0 % If we don't expand the argument now, \skipspaces will get % snagged on things like "@value{foo}". \edef\temp{#1}% \expandafter\skipspaces\temp|\relax } % make a live url in pdf output. \def\pdfurl#1{% \begingroup % it seems we really need yet another set of dummies; have not % tried to figure out what each command should do in the context % of @url. for now, just make @/ a no-op, that's the only one % people have actually reported a problem with. % \normalturnoffactive \def\@{@}% \let\/=\empty \makevalueexpandable % do we want to go so far as to use \indexnofonts instead of just % special-casing \var here? \def\var##1{##1}% % \leavevmode\setcolor{\urlcolor}% \special{pdf:bann << /Border [0 0 0] /Subtype /Link /A << /S /URI /URI (#1) >> >>}% \endgroup} \def\endlink{\setcolor{\maincolor}\special{pdf:eann}} \def\pdfgettoks#1.{\setbox\boxA=\hbox{\toksA={#1.}\toksB={}\maketoks}} \def\addtokens#1#2{\edef\addtoks{\noexpand#1={\the#1#2}}\addtoks} \def\adn#1{\addtokens{\toksC}{#1}\global\countA=1\let\next=\maketoks} \def\poptoks#1#2|ENDTOKS|{\let\first=#1\toksD={#1}\toksA={#2}} \def\maketoks{% \expandafter\poptoks\the\toksA|ENDTOKS|\relax \ifx\first0\adn0 \else\ifx\first1\adn1 \else\ifx\first2\adn2 \else\ifx\first3\adn3 \else\ifx\first4\adn4 \else\ifx\first5\adn5 \else\ifx\first6\adn6 \else\ifx\first7\adn7 \else\ifx\first8\adn8 \else\ifx\first9\adn9 \else \ifnum0=\countA\else\makelink\fi \ifx\first.\let\next=\done\else \let\next=\maketoks \addtokens{\toksB}{\the\toksD} \ifx\first,\addtokens{\toksB}{\space}\fi \fi \fi\fi\fi\fi\fi\fi\fi\fi\fi\fi \next} \def\makelink{\addtokens{\toksB}% {\noexpand\pdflink{\the\toksC}}\toksC={}\global\countA=0} \def\pdflink#1{% \special{pdf:bann << /Border [0 0 0] /Type /Annot /Subtype /Link /A << /S /GoTo /D (#1) >> >>}% \setcolor{\linkcolor}#1\endlink} \def\done{\edef\st{\global\noexpand\toksA={\the\toksB}}\st} % % % @image support % % #1 is image name, #2 width (might be empty/whitespace), #3 height (ditto). \def\doxeteximage#1#2#3{% \def\xeteximagewidth{#2}\setbox0 = \hbox{\ignorespaces #2}% \def\xeteximageheight{#3}\setbox2 = \hbox{\ignorespaces #3}% % % XeTeX (and the PDF format) supports .pdf, .png, .jpg (among % others). Let's try in that order, PDF first since if % someone has a scalable image, presumably better to use that than a % bitmap. \let\xeteximgext=\empty \begingroup \openin 1 #1.pdf \ifeof 1 \openin 1 #1.PDF \ifeof 1 \openin 1 #1.png \ifeof 1 \openin 1 #1.jpg \ifeof 1 \openin 1 #1.jpeg \ifeof 1 \openin 1 #1.JPG \ifeof 1 \errmessage{Could not find image file #1 for XeTeX}% \else \gdef\xeteximgext{JPG}% \fi \else \gdef\xeteximgext{jpeg}% \fi \else \gdef\xeteximgext{jpg}% \fi \else \gdef\xeteximgext{png}% \fi \else \gdef\xeteximgext{PDF}% \fi \else \gdef\xeteximgext{pdf}% \fi \closein 1 \endgroup % \def\xetexpdfext{pdf}% \ifx\xeteximgext\xetexpdfext \XeTeXpdffile "#1".\xeteximgext "" \else \def\xetexpdfext{PDF}% \ifx\xeteximgext\xetexpdfext \XeTeXpdffile "#1".\xeteximgext "" \else \XeTeXpicfile "#1".\xeteximgext "" \fi \fi \ifdim \wd0 >0pt width \xeteximagewidth \fi \ifdim \wd2 >0pt height \xeteximageheight \fi \relax } \fi % \message{fonts,} % Set the baselineskip to #1, and the lineskip and strut size % correspondingly. There is no deep meaning behind these magic numbers % used as factors; they just match (closely enough) what Knuth defined. % \def\lineskipfactor{.08333} \def\strutheightpercent{.70833} \def\strutdepthpercent {.29167} % % can get a sort of poor man's double spacing by redefining this. \def\baselinefactor{1} % \newdimen\textleading \def\setleading#1{% \dimen0 = #1\relax \normalbaselineskip = \baselinefactor\dimen0 \normallineskip = \lineskipfactor\normalbaselineskip \normalbaselines \setbox\strutbox =\hbox{% \vrule width0pt height\strutheightpercent\baselineskip depth \strutdepthpercent \baselineskip }% } % PDF CMaps. See also LaTeX's t1.cmap. % % do nothing with this by default. \expandafter\let\csname cmapOT1\endcsname\gobble \expandafter\let\csname cmapOT1IT\endcsname\gobble \expandafter\let\csname cmapOT1TT\endcsname\gobble % if we are producing pdf, and we have \pdffontattr, then define cmaps. % (\pdffontattr was introduced many years ago, but people still run % older pdftex's; it's easy to conditionalize, so we do.) \ifpdf \ifx\pdffontattr\thisisundefined \else \begingroup \catcode`\^^M=\active \def^^M{^^J}% Output line endings as the ^^J char. \catcode`\%=12 \immediate\pdfobj stream {%!PS-Adobe-3.0 Resource-CMap %%DocumentNeededResources: ProcSet (CIDInit) %%IncludeResource: ProcSet (CIDInit) %%BeginResource: CMap (TeX-OT1-0) %%Title: (TeX-OT1-0 TeX OT1 0) %%Version: 1.000 %%EndComments /CIDInit /ProcSet findresource begin 12 dict begin begincmap /CIDSystemInfo << /Registry (TeX) /Ordering (OT1) /Supplement 0 >> def /CMapName /TeX-OT1-0 def /CMapType 2 def 1 begincodespacerange <00> <7F> endcodespacerange 8 beginbfrange <00> <01> <0393> <09> <0A> <03A8> <23> <26> <0023> <28> <3B> <0028> <3F> <5B> <003F> <5D> <5E> <005D> <61> <7A> <0061> <7B> <7C> <2013> endbfrange 40 beginbfchar <02> <0398> <03> <039B> <04> <039E> <05> <03A0> <06> <03A3> <07> <03D2> <08> <03A6> <0B> <00660066> <0C> <00660069> <0D> <0066006C> <0E> <006600660069> <0F> <00660066006C> <10> <0131> <11> <0237> <12> <0060> <13> <00B4> <14> <02C7> <15> <02D8> <16> <00AF> <17> <02DA> <18> <00B8> <19> <00DF> <1A> <00E6> <1B> <0153> <1C> <00F8> <1D> <00C6> <1E> <0152> <1F> <00D8> <21> <0021> <22> <201D> <27> <2019> <3C> <00A1> <3D> <003D> <3E> <00BF> <5C> <201C> <5F> <02D9> <60> <2018> <7D> <02DD> <7E> <007E> <7F> <00A8> endbfchar endcmap CMapName currentdict /CMap defineresource pop end end %%EndResource %%EOF }\endgroup \expandafter\edef\csname cmapOT1\endcsname#1{% \pdffontattr#1{/ToUnicode \the\pdflastobj\space 0 R}% }% % % \cmapOT1IT \begingroup \catcode`\^^M=\active \def^^M{^^J}% Output line endings as the ^^J char. \catcode`\%=12 \immediate\pdfobj stream {%!PS-Adobe-3.0 Resource-CMap %%DocumentNeededResources: ProcSet (CIDInit) %%IncludeResource: ProcSet (CIDInit) %%BeginResource: CMap (TeX-OT1IT-0) %%Title: (TeX-OT1IT-0 TeX OT1IT 0) %%Version: 1.000 %%EndComments /CIDInit /ProcSet findresource begin 12 dict begin begincmap /CIDSystemInfo << /Registry (TeX) /Ordering (OT1IT) /Supplement 0 >> def /CMapName /TeX-OT1IT-0 def /CMapType 2 def 1 begincodespacerange <00> <7F> endcodespacerange 8 beginbfrange <00> <01> <0393> <09> <0A> <03A8> <25> <26> <0025> <28> <3B> <0028> <3F> <5B> <003F> <5D> <5E> <005D> <61> <7A> <0061> <7B> <7C> <2013> endbfrange 42 beginbfchar <02> <0398> <03> <039B> <04> <039E> <05> <03A0> <06> <03A3> <07> <03D2> <08> <03A6> <0B> <00660066> <0C> <00660069> <0D> <0066006C> <0E> <006600660069> <0F> <00660066006C> <10> <0131> <11> <0237> <12> <0060> <13> <00B4> <14> <02C7> <15> <02D8> <16> <00AF> <17> <02DA> <18> <00B8> <19> <00DF> <1A> <00E6> <1B> <0153> <1C> <00F8> <1D> <00C6> <1E> <0152> <1F> <00D8> <21> <0021> <22> <201D> <23> <0023> <24> <00A3> <27> <2019> <3C> <00A1> <3D> <003D> <3E> <00BF> <5C> <201C> <5F> <02D9> <60> <2018> <7D> <02DD> <7E> <007E> <7F> <00A8> endbfchar endcmap CMapName currentdict /CMap defineresource pop end end %%EndResource %%EOF }\endgroup \expandafter\edef\csname cmapOT1IT\endcsname#1{% \pdffontattr#1{/ToUnicode \the\pdflastobj\space 0 R}% }% % % \cmapOT1TT \begingroup \catcode`\^^M=\active \def^^M{^^J}% Output line endings as the ^^J char. \catcode`\%=12 \immediate\pdfobj stream {%!PS-Adobe-3.0 Resource-CMap %%DocumentNeededResources: ProcSet (CIDInit) %%IncludeResource: ProcSet (CIDInit) %%BeginResource: CMap (TeX-OT1TT-0) %%Title: (TeX-OT1TT-0 TeX OT1TT 0) %%Version: 1.000 %%EndComments /CIDInit /ProcSet findresource begin 12 dict begin begincmap /CIDSystemInfo << /Registry (TeX) /Ordering (OT1TT) /Supplement 0 >> def /CMapName /TeX-OT1TT-0 def /CMapType 2 def 1 begincodespacerange <00> <7F> endcodespacerange 5 beginbfrange <00> <01> <0393> <09> <0A> <03A8> <21> <26> <0021> <28> <5F> <0028> <61> <7E> <0061> endbfrange 32 beginbfchar <02> <0398> <03> <039B> <04> <039E> <05> <03A0> <06> <03A3> <07> <03D2> <08> <03A6> <0B> <2191> <0C> <2193> <0D> <0027> <0E> <00A1> <0F> <00BF> <10> <0131> <11> <0237> <12> <0060> <13> <00B4> <14> <02C7> <15> <02D8> <16> <00AF> <17> <02DA> <18> <00B8> <19> <00DF> <1A> <00E6> <1B> <0153> <1C> <00F8> <1D> <00C6> <1E> <0152> <1F> <00D8> <20> <2423> <27> <2019> <60> <2018> <7F> <00A8> endbfchar endcmap CMapName currentdict /CMap defineresource pop end end %%EndResource %%EOF }\endgroup \expandafter\edef\csname cmapOT1TT\endcsname#1{% \pdffontattr#1{/ToUnicode \the\pdflastobj\space 0 R}% }% \fi\fi % Set the font macro #1 to the font named \fontprefix#2. % #3 is the font's design size, #4 is a scale factor, #5 is the CMap % encoding (only OT1, OT1IT and OT1TT are allowed, or empty to omit). % Example: % #1 = \textrm % #2 = \rmshape % #3 = 10 % #4 = \mainmagstep % #5 = OT1 % \def\setfont#1#2#3#4#5{% \font#1=\fontprefix#2#3 scaled #4 \csname cmap#5\endcsname#1% } % This is what gets called when #5 of \setfont is empty. \let\cmap\gobble % % (end of cmaps) % Use cm as the default font prefix. % To specify the font prefix, you must define \fontprefix % before you read in texinfo.tex. \ifx\fontprefix\thisisundefined \def\fontprefix{cm} \fi % Support font families that don't use the same naming scheme as CM. \def\rmshape{r} \def\rmbshape{bx} % where the normal face is bold \def\bfshape{b} \def\bxshape{bx} \def\ttshape{tt} \def\ttbshape{tt} \def\ttslshape{sltt} \def\itshape{ti} \def\itbshape{bxti} \def\slshape{sl} \def\slbshape{bxsl} \def\sfshape{ss} \def\sfbshape{ss} \def\scshape{csc} \def\scbshape{csc} % Definitions for a main text size of 11pt. (The default in Texinfo.) % \def\definetextfontsizexi{% % Text fonts (11.2pt, magstep1). \def\textnominalsize{11pt} \edef\mainmagstep{\magstephalf} \setfont\textrm\rmshape{10}{\mainmagstep}{OT1} \setfont\texttt\ttshape{10}{\mainmagstep}{OT1TT} \setfont\textbf\bfshape{10}{\mainmagstep}{OT1} \setfont\textit\itshape{10}{\mainmagstep}{OT1IT} \setfont\textsl\slshape{10}{\mainmagstep}{OT1} \setfont\textsf\sfshape{10}{\mainmagstep}{OT1} \setfont\textsc\scshape{10}{\mainmagstep}{OT1} \setfont\textttsl\ttslshape{10}{\mainmagstep}{OT1TT} \font\texti=cmmi10 scaled \mainmagstep \font\textsy=cmsy10 scaled \mainmagstep \def\textecsize{1095} % A few fonts for @defun names and args. \setfont\defbf\bfshape{10}{\magstep1}{OT1} \setfont\deftt\ttshape{10}{\magstep1}{OT1TT} \setfont\defsl\slshape{10}{\magstep1}{OT1TT} \setfont\defttsl\ttslshape{10}{\magstep1}{OT1TT} \def\df{\let\ttfont=\deftt \let\bffont = \defbf \let\ttslfont=\defttsl \let\slfont=\defsl \bf} % Fonts for indices, footnotes, small examples (9pt). \def\smallnominalsize{9pt} \setfont\smallrm\rmshape{9}{1000}{OT1} \setfont\smalltt\ttshape{9}{1000}{OT1TT} \setfont\smallbf\bfshape{10}{900}{OT1} \setfont\smallit\itshape{9}{1000}{OT1IT} \setfont\smallsl\slshape{9}{1000}{OT1} \setfont\smallsf\sfshape{9}{1000}{OT1} \setfont\smallsc\scshape{10}{900}{OT1} \setfont\smallttsl\ttslshape{10}{900}{OT1TT} \font\smalli=cmmi9 \font\smallsy=cmsy9 \def\smallecsize{0900} % Fonts for small examples (8pt). \def\smallernominalsize{8pt} \setfont\smallerrm\rmshape{8}{1000}{OT1} \setfont\smallertt\ttshape{8}{1000}{OT1TT} \setfont\smallerbf\bfshape{10}{800}{OT1} \setfont\smallerit\itshape{8}{1000}{OT1IT} \setfont\smallersl\slshape{8}{1000}{OT1} \setfont\smallersf\sfshape{8}{1000}{OT1} \setfont\smallersc\scshape{10}{800}{OT1} \setfont\smallerttsl\ttslshape{10}{800}{OT1TT} \font\smalleri=cmmi8 \font\smallersy=cmsy8 \def\smallerecsize{0800} % Fonts for title page (20.4pt): \def\titlenominalsize{20pt} \setfont\titlerm\rmbshape{12}{\magstep3}{OT1} \setfont\titleit\itbshape{10}{\magstep4}{OT1IT} \setfont\titlesl\slbshape{10}{\magstep4}{OT1} \setfont\titlett\ttbshape{12}{\magstep3}{OT1TT} \setfont\titlettsl\ttslshape{10}{\magstep4}{OT1TT} \setfont\titlesf\sfbshape{17}{\magstep1}{OT1} \let\titlebf=\titlerm \setfont\titlesc\scbshape{10}{\magstep4}{OT1} \font\titlei=cmmi12 scaled \magstep3 \font\titlesy=cmsy10 scaled \magstep4 \def\titleecsize{2074} % Chapter (and unnumbered) fonts (17.28pt). \def\chapnominalsize{17pt} \setfont\chaprm\rmbshape{12}{\magstep2}{OT1} \setfont\chapit\itbshape{10}{\magstep3}{OT1IT} \setfont\chapsl\slbshape{10}{\magstep3}{OT1} \setfont\chaptt\ttbshape{12}{\magstep2}{OT1TT} \setfont\chapttsl\ttslshape{10}{\magstep3}{OT1TT} \setfont\chapsf\sfbshape{17}{1000}{OT1} \let\chapbf=\chaprm \setfont\chapsc\scbshape{10}{\magstep3}{OT1} \font\chapi=cmmi12 scaled \magstep2 \font\chapsy=cmsy10 scaled \magstep3 \def\chapecsize{1728} % Section fonts (14.4pt). \def\secnominalsize{14pt} \setfont\secrm\rmbshape{12}{\magstep1}{OT1} \setfont\secrmnotbold\rmshape{12}{\magstep1}{OT1} \setfont\secit\itbshape{10}{\magstep2}{OT1IT} \setfont\secsl\slbshape{10}{\magstep2}{OT1} \setfont\sectt\ttbshape{12}{\magstep1}{OT1TT} \setfont\secttsl\ttslshape{10}{\magstep2}{OT1TT} \setfont\secsf\sfbshape{12}{\magstep1}{OT1} \let\secbf\secrm \setfont\secsc\scbshape{10}{\magstep2}{OT1} \font\seci=cmmi12 scaled \magstep1 \font\secsy=cmsy10 scaled \magstep2 \def\sececsize{1440} % Subsection fonts (13.15pt). \def\ssecnominalsize{13pt} \setfont\ssecrm\rmbshape{12}{\magstephalf}{OT1} \setfont\ssecit\itbshape{10}{1315}{OT1IT} \setfont\ssecsl\slbshape{10}{1315}{OT1} \setfont\ssectt\ttbshape{12}{\magstephalf}{OT1TT} \setfont\ssecttsl\ttslshape{10}{1315}{OT1TT} \setfont\ssecsf\sfbshape{12}{\magstephalf}{OT1} \let\ssecbf\ssecrm \setfont\ssecsc\scbshape{10}{1315}{OT1} \font\sseci=cmmi12 scaled \magstephalf \font\ssecsy=cmsy10 scaled 1315 \def\ssececsize{1200} % Reduced fonts for @acronym in text (10pt). \def\reducednominalsize{10pt} \setfont\reducedrm\rmshape{10}{1000}{OT1} \setfont\reducedtt\ttshape{10}{1000}{OT1TT} \setfont\reducedbf\bfshape{10}{1000}{OT1} \setfont\reducedit\itshape{10}{1000}{OT1IT} \setfont\reducedsl\slshape{10}{1000}{OT1} \setfont\reducedsf\sfshape{10}{1000}{OT1} \setfont\reducedsc\scshape{10}{1000}{OT1} \setfont\reducedttsl\ttslshape{10}{1000}{OT1TT} \font\reducedi=cmmi10 \font\reducedsy=cmsy10 \def\reducedecsize{1000} \textleading = 13.2pt % line spacing for 11pt CM \textfonts % reset the current fonts \rm } % end of 11pt text font size definitions, \definetextfontsizexi % Definitions to make the main text be 10pt Computer Modern, with % section, chapter, etc., sizes following suit. This is for the GNU % Press printing of the Emacs 22 manual. Maybe other manuals in the % future. Used with @smallbook, which sets the leading to 12pt. % \def\definetextfontsizex{% % Text fonts (10pt). \def\textnominalsize{10pt} \edef\mainmagstep{1000} \setfont\textrm\rmshape{10}{\mainmagstep}{OT1} \setfont\texttt\ttshape{10}{\mainmagstep}{OT1TT} \setfont\textbf\bfshape{10}{\mainmagstep}{OT1} \setfont\textit\itshape{10}{\mainmagstep}{OT1IT} \setfont\textsl\slshape{10}{\mainmagstep}{OT1} \setfont\textsf\sfshape{10}{\mainmagstep}{OT1} \setfont\textsc\scshape{10}{\mainmagstep}{OT1} \setfont\textttsl\ttslshape{10}{\mainmagstep}{OT1TT} \font\texti=cmmi10 scaled \mainmagstep \font\textsy=cmsy10 scaled \mainmagstep \def\textecsize{1000} % A few fonts for @defun names and args. \setfont\defbf\bfshape{10}{\magstephalf}{OT1} \setfont\deftt\ttshape{10}{\magstephalf}{OT1TT} \setfont\defsl\slshape{10}{\magstephalf}{OT1TT} \setfont\defttsl\ttslshape{10}{\magstephalf}{OT1TT} \def\df{\let\ttfont=\deftt \let\bffont = \defbf \let\slfont=\defsl \let\ttslfont=\defttsl \bf} % Fonts for indices, footnotes, small examples (9pt). \def\smallnominalsize{9pt} \setfont\smallrm\rmshape{9}{1000}{OT1} \setfont\smalltt\ttshape{9}{1000}{OT1TT} \setfont\smallbf\bfshape{10}{900}{OT1} \setfont\smallit\itshape{9}{1000}{OT1IT} \setfont\smallsl\slshape{9}{1000}{OT1} \setfont\smallsf\sfshape{9}{1000}{OT1} \setfont\smallsc\scshape{10}{900}{OT1} \setfont\smallttsl\ttslshape{10}{900}{OT1TT} \font\smalli=cmmi9 \font\smallsy=cmsy9 \def\smallecsize{0900} % Fonts for small examples (8pt). \def\smallernominalsize{8pt} \setfont\smallerrm\rmshape{8}{1000}{OT1} \setfont\smallertt\ttshape{8}{1000}{OT1TT} \setfont\smallerbf\bfshape{10}{800}{OT1} \setfont\smallerit\itshape{8}{1000}{OT1IT} \setfont\smallersl\slshape{8}{1000}{OT1} \setfont\smallersf\sfshape{8}{1000}{OT1} \setfont\smallersc\scshape{10}{800}{OT1} \setfont\smallerttsl\ttslshape{10}{800}{OT1TT} \font\smalleri=cmmi8 \font\smallersy=cmsy8 \def\smallerecsize{0800} % Fonts for title page (20.4pt): \def\titlenominalsize{20pt} \setfont\titlerm\rmbshape{12}{\magstep3}{OT1} \setfont\titleit\itbshape{10}{\magstep4}{OT1IT} \setfont\titlesl\slbshape{10}{\magstep4}{OT1} \setfont\titlett\ttbshape{12}{\magstep3}{OT1TT} \setfont\titlettsl\ttslshape{10}{\magstep4}{OT1TT} \setfont\titlesf\sfbshape{17}{\magstep1}{OT1} \let\titlebf=\titlerm \setfont\titlesc\scbshape{10}{\magstep4}{OT1} \font\titlei=cmmi12 scaled \magstep3 \font\titlesy=cmsy10 scaled \magstep4 \def\titleecsize{2074} % Chapter fonts (14.4pt). \def\chapnominalsize{14pt} \setfont\chaprm\rmbshape{12}{\magstep1}{OT1} \setfont\chapit\itbshape{10}{\magstep2}{OT1IT} \setfont\chapsl\slbshape{10}{\magstep2}{OT1} \setfont\chaptt\ttbshape{12}{\magstep1}{OT1TT} \setfont\chapttsl\ttslshape{10}{\magstep2}{OT1TT} \setfont\chapsf\sfbshape{12}{\magstep1}{OT1} \let\chapbf\chaprm \setfont\chapsc\scbshape{10}{\magstep2}{OT1} \font\chapi=cmmi12 scaled \magstep1 \font\chapsy=cmsy10 scaled \magstep2 \def\chapecsize{1440} % Section fonts (12pt). \def\secnominalsize{12pt} \setfont\secrm\rmbshape{12}{1000}{OT1} \setfont\secit\itbshape{10}{\magstep1}{OT1IT} \setfont\secsl\slbshape{10}{\magstep1}{OT1} \setfont\sectt\ttbshape{12}{1000}{OT1TT} \setfont\secttsl\ttslshape{10}{\magstep1}{OT1TT} \setfont\secsf\sfbshape{12}{1000}{OT1} \let\secbf\secrm \setfont\secsc\scbshape{10}{\magstep1}{OT1} \font\seci=cmmi12 \font\secsy=cmsy10 scaled \magstep1 \def\sececsize{1200} % Subsection fonts (10pt). \def\ssecnominalsize{10pt} \setfont\ssecrm\rmbshape{10}{1000}{OT1} \setfont\ssecit\itbshape{10}{1000}{OT1IT} \setfont\ssecsl\slbshape{10}{1000}{OT1} \setfont\ssectt\ttbshape{10}{1000}{OT1TT} \setfont\ssecttsl\ttslshape{10}{1000}{OT1TT} \setfont\ssecsf\sfbshape{10}{1000}{OT1} \let\ssecbf\ssecrm \setfont\ssecsc\scbshape{10}{1000}{OT1} \font\sseci=cmmi10 \font\ssecsy=cmsy10 \def\ssececsize{1000} % Reduced fonts for @acronym in text (9pt). \def\reducednominalsize{9pt} \setfont\reducedrm\rmshape{9}{1000}{OT1} \setfont\reducedtt\ttshape{9}{1000}{OT1TT} \setfont\reducedbf\bfshape{10}{900}{OT1} \setfont\reducedit\itshape{9}{1000}{OT1IT} \setfont\reducedsl\slshape{9}{1000}{OT1} \setfont\reducedsf\sfshape{9}{1000}{OT1} \setfont\reducedsc\scshape{10}{900}{OT1} \setfont\reducedttsl\ttslshape{10}{900}{OT1TT} \font\reducedi=cmmi9 \font\reducedsy=cmsy9 \def\reducedecsize{0900} \divide\parskip by 2 % reduce space between paragraphs \textleading = 12pt % line spacing for 10pt CM \textfonts % reset the current fonts \rm } % end of 10pt text font size definitions, \definetextfontsizex % Fonts for short table of contents. \setfont\shortcontrm\rmshape{12}{1000}{OT1} \setfont\shortcontbf\bfshape{10}{\magstep1}{OT1} % no cmb12 \setfont\shortcontsl\slshape{12}{1000}{OT1} \setfont\shortconttt\ttshape{12}{1000}{OT1TT} % We provide the user-level command % @fonttextsize 10 % (or 11) to redefine the text font size. pt is assumed. % \def\xiword{11} \def\xword{10} \def\xwordpt{10pt} % \parseargdef\fonttextsize{% \def\textsizearg{#1}% %\wlog{doing @fonttextsize \textsizearg}% % % Set \globaldefs so that documents can use this inside @tex, since % makeinfo 4.8 does not support it, but we need it nonetheless. % \begingroup \globaldefs=1 \ifx\textsizearg\xword \definetextfontsizex \else \ifx\textsizearg\xiword \definetextfontsizexi \else \errhelp=\EMsimple \errmessage{@fonttextsize only supports `10' or `11', not `\textsizearg'} \fi\fi \endgroup } % % Change the current font style to #1, remembering it in \curfontstyle. % For now, we do not accumulate font styles: @b{@i{foo}} prints foo in % italics, not bold italics. % \def\setfontstyle#1{% \def\curfontstyle{#1}% not as a control sequence, because we are \edef'd. \csname #1font\endcsname % change the current font } \def\rm{\fam=0 \setfontstyle{rm}} \def\it{\fam=\itfam \setfontstyle{it}} \def\sl{\fam=\slfam \setfontstyle{sl}} \def\bf{\fam=\bffam \setfontstyle{bf}}\def\bfstylename{bf} \def\tt{\fam=\ttfam \setfontstyle{tt}} % Texinfo sort of supports the sans serif font style, which plain TeX does not. % So we set up a \sf. \newfam\sffam \def\sf{\fam=\sffam \setfontstyle{sf}} % We don't need math for this font style. \def\ttsl{\setfontstyle{ttsl}} % In order for the font changes to affect most math symbols and letters, % we have to define the \textfont of the standard families. We don't % bother to reset \scriptfont and \scriptscriptfont; awaiting user need. % \def\resetmathfonts{% \textfont0=\rmfont \textfont1=\ifont \textfont2=\syfont \textfont\itfam=\itfont \textfont\slfam=\slfont \textfont\bffam=\bffont \textfont\ttfam=\ttfont \textfont\sffam=\sffont } % % The font-changing commands (all called \...fonts) redefine the meanings % of \STYLEfont, instead of just \STYLE. We do this because \STYLE needs % to also set the current \fam for math mode. Our \STYLE (e.g., \rm) % commands hardwire \STYLEfont to set the current font. % % Each font-changing command also sets the names \lsize (one size lower) % and \lllsize (three sizes lower). These relative commands are used % in, e.g., the LaTeX logo and acronyms. % % This all needs generalizing, badly. % \def\assignfonts#1{% \expandafter\let\expandafter\rmfont\csname #1rm\endcsname \expandafter\let\expandafter\itfont\csname #1it\endcsname \expandafter\let\expandafter\slfont\csname #1sl\endcsname \expandafter\let\expandafter\bffont\csname #1bf\endcsname \expandafter\let\expandafter\ttfont\csname #1tt\endcsname \expandafter\let\expandafter\smallcaps\csname #1sc\endcsname \expandafter\let\expandafter\sffont \csname #1sf\endcsname \expandafter\let\expandafter\ifont \csname #1i\endcsname \expandafter\let\expandafter\syfont \csname #1sy\endcsname \expandafter\let\expandafter\ttslfont\csname #1ttsl\endcsname } \newif\ifrmisbold % Select smaller font size with the current style. Used to change font size % in, e.g., the LaTeX logo and acronyms. If we are using bold fonts for % normal roman text, also use bold fonts for roman text in the smaller size. \def\switchtolllsize{% \expandafter\assignfonts\expandafter{\lllsize}% \ifrmisbold \let\rmfont\bffont \fi \csname\curfontstyle\endcsname }% \def\switchtolsize{% \expandafter\assignfonts\expandafter{\lsize}% \ifrmisbold \let\rmfont\bffont \fi \csname\curfontstyle\endcsname }% \def\definefontsetatsize#1#2#3#4#5{% \expandafter\def\csname #1fonts\endcsname{% \def\curfontsize{#1}% \def\lsize{#2}\def\lllsize{#3}% \csname rmisbold#5\endcsname \assignfonts{#1}% \resetmathfonts \setleading{#4}% }} \definefontsetatsize{text} {reduced}{smaller}{\textleading}{false} \definefontsetatsize{title} {chap} {subsec} {27pt} {true} \definefontsetatsize{chap} {sec} {text} {19pt} {true} \definefontsetatsize{sec} {subsec} {reduced}{17pt} {true} \definefontsetatsize{ssec} {text} {small} {15pt} {true} \definefontsetatsize{reduced}{small} {smaller}{10.5pt}{false} \definefontsetatsize{small} {smaller}{smaller}{10.5pt}{false} \definefontsetatsize{smaller}{smaller}{smaller}{9.5pt} {false} \def\titlefont#1{{\titlefonts\rm #1}} \let\subsecfonts = \ssecfonts \let\subsubsecfonts = \ssecfonts % Define these just so they can be easily changed for other fonts. \def\angleleft{$\langle$} \def\angleright{$\rangle$} % Set the fonts to use with the @small... environments. \let\smallexamplefonts = \smallfonts % About \smallexamplefonts. If we use \smallfonts (9pt), @smallexample % can fit this many characters: % 8.5x11=86 smallbook=72 a4=90 a5=69 % If we use \scriptfonts (8pt), then we can fit this many characters: % 8.5x11=90+ smallbook=80 a4=90+ a5=77 % For me, subjectively, the few extra characters that fit aren't worth % the additional smallness of 8pt. So I'm making the default 9pt. % % By the way, for comparison, here's what fits with @example (10pt): % 8.5x11=71 smallbook=60 a4=75 a5=58 % --karl, 24jan03. % Set up the default fonts, so we can use them for creating boxes. % \definetextfontsizexi \message{markup,} % Check if we are currently using a typewriter font. Since all the % Computer Modern typewriter fonts have zero interword stretch (and % shrink), and it is reasonable to expect all typewriter fonts to have % this property, we can check that font parameter. % \def\ifmonospace{\ifdim\fontdimen3\font=0pt } % Markup style infrastructure. \defmarkupstylesetup\INITMACRO will % define and register \INITMACRO to be called on markup style changes. % \INITMACRO can check \currentmarkupstyle for the innermost % style and the set of \ifmarkupSTYLE switches for all styles % currently in effect. \newif\ifmarkupvar \newif\ifmarkupsamp \newif\ifmarkupkey %\newif\ifmarkupfile % @file == @samp. %\newif\ifmarkupoption % @option == @samp. \newif\ifmarkupcode \newif\ifmarkupkbd %\newif\ifmarkupenv % @env == @code. %\newif\ifmarkupcommand % @command == @code. \newif\ifmarkuptex % @tex (and part of @math, for now). \newif\ifmarkupexample \newif\ifmarkupverb \newif\ifmarkupverbatim \let\currentmarkupstyle\empty \def\setupmarkupstyle#1{% \csname markup#1true\endcsname \def\currentmarkupstyle{#1}% \markupstylesetup } \let\markupstylesetup\empty \def\defmarkupstylesetup#1{% \expandafter\def\expandafter\markupstylesetup \expandafter{\markupstylesetup #1}% \def#1% } % Markup style setup for left and right quotes. \defmarkupstylesetup\markupsetuplq{% \expandafter\let\expandafter \temp \csname markupsetuplq\currentmarkupstyle\endcsname \ifx\temp\relax \markupsetuplqdefault \else \temp \fi } \defmarkupstylesetup\markupsetuprq{% \expandafter\let\expandafter \temp \csname markupsetuprq\currentmarkupstyle\endcsname \ifx\temp\relax \markupsetuprqdefault \else \temp \fi } { \catcode`\'=\active \catcode`\`=\active \gdef\markupsetuplqdefault{\let`\lq} \gdef\markupsetuprqdefault{\let'\rq} \gdef\markupsetcodequoteleft{\let`\codequoteleft} \gdef\markupsetcodequoteright{\let'\codequoteright} } \let\markupsetuplqcode \markupsetcodequoteleft \let\markupsetuprqcode \markupsetcodequoteright % \let\markupsetuplqexample \markupsetcodequoteleft \let\markupsetuprqexample \markupsetcodequoteright % \let\markupsetuplqkbd \markupsetcodequoteleft \let\markupsetuprqkbd \markupsetcodequoteright % \let\markupsetuplqsamp \markupsetcodequoteleft \let\markupsetuprqsamp \markupsetcodequoteright % \let\markupsetuplqverb \markupsetcodequoteleft \let\markupsetuprqverb \markupsetcodequoteright % \let\markupsetuplqverbatim \markupsetcodequoteleft \let\markupsetuprqverbatim \markupsetcodequoteright % Allow an option to not use regular directed right quote/apostrophe % (char 0x27), but instead the undirected quote from cmtt (char 0x0d). % The undirected quote is ugly, so don't make it the default, but it % works for pasting with more pdf viewers (at least evince), the % lilypond developers report. xpdf does work with the regular 0x27. % \def\codequoteright{% \expandafter\ifx\csname SETtxicodequoteundirected\endcsname\relax \expandafter\ifx\csname SETcodequoteundirected\endcsname\relax '% \else \char'15 \fi \else \char'15 \fi } % % and a similar option for the left quote char vs. a grave accent. % Modern fonts display ASCII 0x60 as a grave accent, so some people like % the code environments to do likewise. % \def\codequoteleft{% \expandafter\ifx\csname SETtxicodequotebacktick\endcsname\relax \expandafter\ifx\csname SETcodequotebacktick\endcsname\relax % [Knuth] pp. 380,381,391 % \relax disables Spanish ligatures ?` and !` of \tt font. \relax`% \else \char'22 \fi \else \char'22 \fi } % Commands to set the quote options. % \parseargdef\codequoteundirected{% \def\temp{#1}% \ifx\temp\onword \expandafter\let\csname SETtxicodequoteundirected\endcsname = t% \else\ifx\temp\offword \expandafter\let\csname SETtxicodequoteundirected\endcsname = \relax \else \errhelp = \EMsimple \errmessage{Unknown @codequoteundirected value `\temp', must be on|off}% \fi\fi } % \parseargdef\codequotebacktick{% \def\temp{#1}% \ifx\temp\onword \expandafter\let\csname SETtxicodequotebacktick\endcsname = t% \else\ifx\temp\offword \expandafter\let\csname SETtxicodequotebacktick\endcsname = \relax \else \errhelp = \EMsimple \errmessage{Unknown @codequotebacktick value `\temp', must be on|off}% \fi\fi } % [Knuth] pp. 380,381,391, disable Spanish ligatures ?` and !` of \tt font. \def\noligaturesquoteleft{\relax\lq} % Count depth in font-changes, for error checks \newcount\fontdepth \fontdepth=0 % Font commands. % #1 is the font command (\sl or \it), #2 is the text to slant. % If we are in a monospaced environment, however, 1) always use \ttsl, % and 2) do not add an italic correction. \def\dosmartslant#1#2{% \ifusingtt {{\ttsl #2}\let\next=\relax}% {\def\next{{#1#2}\futurelet\next\smartitaliccorrection}}% \next } \def\smartslanted{\dosmartslant\sl} \def\smartitalic{\dosmartslant\it} % Output an italic correction unless \next (presumed to be the following % character) is such as not to need one. \def\smartitaliccorrection{% \ifx\next,% \else\ifx\next-% \else\ifx\next.% \else\ifx\next\.% \else\ifx\next\comma% \else\ptexslash \fi\fi\fi\fi\fi \aftersmartic } % Unconditional use \ttsl, and no ic. @var is set to this for defuns. \def\ttslanted#1{{\ttsl #1}} % @cite is like \smartslanted except unconditionally use \sl. We never want % ttsl for book titles, do we? \def\cite#1{{\sl #1}\futurelet\next\smartitaliccorrection} \def\aftersmartic{} \def\var#1{% \let\saveaftersmartic = \aftersmartic \def\aftersmartic{\null\let\aftersmartic=\saveaftersmartic}% \smartslanted{#1}% } \let\i=\smartitalic \let\slanted=\smartslanted \let\dfn=\smartslanted \let\emph=\smartitalic % Explicit font changes: @r, @sc, undocumented @ii. \def\r#1{{\rm #1}} % roman font \def\sc#1{{\smallcaps#1}} % smallcaps font \def\ii#1{{\it #1}} % italic font % @b, explicit bold. Also @strong. \def\b#1{{\bf #1}} \let\strong=\b % @sansserif, explicit sans. \def\sansserif#1{{\sf #1}} % We can't just use \exhyphenpenalty, because that only has effect at % the end of a paragraph. Restore normal hyphenation at the end of the % group within which \nohyphenation is presumably called. % \def\nohyphenation{\hyphenchar\font = -1 \aftergroup\restorehyphenation} \def\restorehyphenation{\hyphenchar\font = `- } % Set sfcode to normal for the chars that usually have another value. % Can't use plain's \frenchspacing because it uses the `\x notation, and % sometimes \x has an active definition that messes things up. % \catcode`@=11 \def\plainfrenchspacing{% \sfcode`\.=\@m \sfcode`\?=\@m \sfcode`\!=\@m \sfcode`\:=\@m \sfcode`\;=\@m \sfcode`\,=\@m \def\endofsentencespacefactor{1000}% for @. and friends } \def\plainnonfrenchspacing{% \sfcode`\.3000\sfcode`\?3000\sfcode`\!3000 \sfcode`\:2000\sfcode`\;1500\sfcode`\,1250 \def\endofsentencespacefactor{3000}% for @. and friends } \catcode`@=\other \def\endofsentencespacefactor{3000}% default % @t, explicit typewriter. \def\t#1{% {\tt \rawbackslash \plainfrenchspacing #1}% \null } % @samp. \def\samp#1{{\setupmarkupstyle{samp}\lq\tclose{#1}\rq\null}} % @indicateurl is \samp, that is, with quotes. \let\indicateurl=\samp % @code (and similar) prints in typewriter, but with spaces the same % size as normal in the surrounding text, without hyphenation, etc. % This is a subroutine for that. \def\tclose#1{% {% % Change normal interword space to be same as for the current font. \spaceskip = \fontdimen2\font % % Switch to typewriter. \tt % % But `\ ' produces the large typewriter interword space. \def\ {{\spaceskip = 0pt{} }}% % % Turn off hyphenation. \nohyphenation % \rawbackslash \plainfrenchspacing #1% }% \null % reset spacefactor to 1000 } % We *must* turn on hyphenation at `-' and `_' in @code. % (But see \codedashfinish below.) % Otherwise, it is too hard to avoid overfull hboxes % in the Emacs manual, the Library manual, etc. % % Unfortunately, TeX uses one parameter (\hyphenchar) to control % both hyphenation at - and hyphenation within words. % We must therefore turn them both off (\tclose does that) % and arrange explicitly to hyphenate at a dash. -- rms. { \catcode`\-=\active \catcode`\_=\active \catcode`\'=\active \catcode`\`=\active \global\let'=\rq \global\let`=\lq % default definitions % \global\def\code{\begingroup \setupmarkupstyle{code}% % The following should really be moved into \setupmarkupstyle handlers. \catcode\dashChar=\active \catcode\underChar=\active \ifallowcodebreaks \let-\codedash \let_\codeunder \else \let-\normaldash \let_\realunder \fi % Given -foo (with a single dash), we do not want to allow a break % after the hyphen. \global\let\codedashprev=\codedash % \codex } % \gdef\codedash{\futurelet\next\codedashfinish} \gdef\codedashfinish{% \normaldash % always output the dash character itself. % % Now, output a discretionary to allow a line break, unless % (a) the next character is a -, or % (b) the preceding character is a -. % E.g., given --posix, we do not want to allow a break after either -. % Given --foo-bar, we do want to allow a break between the - and the b. \ifx\next\codedash \else \ifx\codedashprev\codedash \else \discretionary{}{}{}\fi \fi % we need the space after the = for the case when \next itself is a % space token; it would get swallowed otherwise. As in @code{- a}. \global\let\codedashprev= \next } } \def\normaldash{-} % \def\codex #1{\tclose{#1}\endgroup} \def\codeunder{% % this is all so @math{@code{var_name}+1} can work. In math mode, _ % is "active" (mathcode"8000) and \normalunderscore (or \char95, etc.) % will therefore expand the active definition of _, which is us % (inside @code that is), therefore an endless loop. \ifusingtt{\ifmmode \mathchar"075F % class 0=ordinary, family 7=ttfam, pos 0x5F=_. \else\normalunderscore \fi \discretionary{}{}{}}% {\_}% } % An additional complication: the above will allow breaks after, e.g., % each of the four underscores in __typeof__. This is bad. % @allowcodebreaks provides a document-level way to turn breaking at - % and _ on and off. % \newif\ifallowcodebreaks \allowcodebreakstrue \def\keywordtrue{true} \def\keywordfalse{false} \parseargdef\allowcodebreaks{% \def\txiarg{#1}% \ifx\txiarg\keywordtrue \allowcodebreakstrue \else\ifx\txiarg\keywordfalse \allowcodebreaksfalse \else \errhelp = \EMsimple \errmessage{Unknown @allowcodebreaks option `\txiarg', must be true|false}% \fi\fi } % For @command, @env, @file, @option quotes seem unnecessary, % so use \code rather than \samp. \let\command=\code \let\env=\code \let\file=\code \let\option=\code % @uref (abbreviation for `urlref') aka @url takes an optional % (comma-separated) second argument specifying the text to display and % an optional third arg as text to display instead of (rather than in % addition to) the url itself. First (mandatory) arg is the url. % TeX-only option to allow changing PDF output to show only the second % arg (if given), and not the url (which is then just the link target). \newif\ifurefurlonlylink % The main macro is \urefbreak, which allows breaking at expected % places within the url. (There used to be another version, which % didn't support automatic breaking.) \def\urefbreak{\begingroup \urefcatcodes \dourefbreak} \let\uref=\urefbreak % \def\dourefbreak#1{\urefbreakfinish #1,,,\finish} \def\urefbreakfinish#1,#2,#3,#4\finish{% doesn't work in @example \unsepspaces \pdfurl{#1}% \setbox0 = \hbox{\ignorespaces #3}% \ifdim\wd0 > 0pt \unhbox0 % third arg given, show only that \else \setbox0 = \hbox{\ignorespaces #2}% look for second arg \ifdim\wd0 > 0pt \ifpdf % For pdfTeX and LuaTeX \ifurefurlonlylink % PDF plus option to not display url, show just arg \unhbox0 \else % PDF, normally display both arg and url for consistency, % visibility, if the pdf is eventually used to print, etc. \unhbox0\ (\urefcode{#1})% \fi \else \ifx\XeTeXrevision\thisisundefined \unhbox0\ (\urefcode{#1})% DVI, always show arg and url \else % For XeTeX \ifurefurlonlylink % PDF plus option to not display url, show just arg \unhbox0 \else % PDF, normally display both arg and url for consistency, % visibility, if the pdf is eventually used to print, etc. \unhbox0\ (\urefcode{#1})% \fi \fi \fi \else \urefcode{#1}% only url given, so show it \fi \fi \endlink \endgroup} % Allow line breaks around only a few characters (only). \def\urefcatcodes{% \catcode`\&=\active \catcode`\.=\active \catcode`\#=\active \catcode`\?=\active \catcode`\/=\active } { \urefcatcodes % \global\def\urefcode{\begingroup \setupmarkupstyle{code}% \urefcatcodes \let&\urefcodeamp \let.\urefcodedot \let#\urefcodehash \let?\urefcodequest \let/\urefcodeslash \codex } % % By default, they are just regular characters. \global\def&{\normalamp} \global\def.{\normaldot} \global\def#{\normalhash} \global\def?{\normalquest} \global\def/{\normalslash} } % we put a little stretch before and after the breakable chars, to help % line breaking of long url's. The unequal skips make look better in % cmtt at least, especially for dots. \def\urefprestretchamount{.13em} \def\urefpoststretchamount{.1em} \def\urefprestretch{\urefprebreak \hskip0pt plus\urefprestretchamount\relax} \def\urefpoststretch{\urefpostbreak \hskip0pt plus\urefprestretchamount\relax} % \def\urefcodeamp{\urefprestretch \&\urefpoststretch} \def\urefcodedot{\urefprestretch .\urefpoststretch} \def\urefcodehash{\urefprestretch \#\urefpoststretch} \def\urefcodequest{\urefprestretch ?\urefpoststretch} \def\urefcodeslash{\futurelet\next\urefcodeslashfinish} { \catcode`\/=\active \global\def\urefcodeslashfinish{% \urefprestretch \slashChar % Allow line break only after the final / in a sequence of % slashes, to avoid line break between the slashes in http://. \ifx\next/\else \urefpoststretch \fi } } % One more complication: by default we'll break after the special % characters, but some people like to break before the special chars, so % allow that. Also allow no breaking at all, for manual control. % \parseargdef\urefbreakstyle{% \def\txiarg{#1}% \ifx\txiarg\wordnone \def\urefprebreak{\nobreak}\def\urefpostbreak{\nobreak} \else\ifx\txiarg\wordbefore \def\urefprebreak{\allowbreak}\def\urefpostbreak{\nobreak} \else\ifx\txiarg\wordafter \def\urefprebreak{\nobreak}\def\urefpostbreak{\allowbreak} \else \errhelp = \EMsimple \errmessage{Unknown @urefbreakstyle setting `\txiarg'}% \fi\fi\fi } \def\wordafter{after} \def\wordbefore{before} \def\wordnone{none} \urefbreakstyle after % @url synonym for @uref, since that's how everyone uses it. % \let\url=\uref % rms does not like angle brackets --karl, 17may97. % So now @email is just like @uref, unless we are pdf. % %\def\email#1{\angleleft{\tt #1}\angleright} \ifpdf \def\email#1{\doemail#1,,\finish} \def\doemail#1,#2,#3\finish{\begingroup \unsepspaces \pdfurl{mailto:#1}% \setbox0 = \hbox{\ignorespaces #2}% \ifdim\wd0>0pt\unhbox0\else\code{#1}\fi \endlink \endgroup} \else \ifx\XeTeXrevision\thisisundefined \let\email=\uref \else \def\email#1{\doemail#1,,\finish} \def\doemail#1,#2,#3\finish{\begingroup \unsepspaces \pdfurl{mailto:#1}% \setbox0 = \hbox{\ignorespaces #2}% \ifdim\wd0>0pt\unhbox0\else\code{#1}\fi \endlink \endgroup} \fi \fi % @kbdinputstyle -- arg is `distinct' (@kbd uses slanted tty font always), % `example' (@kbd uses ttsl only inside of @example and friends), % or `code' (@kbd uses normal tty font always). \parseargdef\kbdinputstyle{% \def\txiarg{#1}% \ifx\txiarg\worddistinct \gdef\kbdexamplefont{\ttsl}\gdef\kbdfont{\ttsl}% \else\ifx\txiarg\wordexample \gdef\kbdexamplefont{\ttsl}\gdef\kbdfont{\tt}% \else\ifx\txiarg\wordcode \gdef\kbdexamplefont{\tt}\gdef\kbdfont{\tt}% \else \errhelp = \EMsimple \errmessage{Unknown @kbdinputstyle setting `\txiarg'}% \fi\fi\fi } \def\worddistinct{distinct} \def\wordexample{example} \def\wordcode{code} % Default is `distinct'. \kbdinputstyle distinct % @kbd is like @code, except that if the argument is just one @key command, % then @kbd has no effect. \def\kbd#1{{\def\look{#1}\expandafter\kbdsub\look??\par}} \def\xkey{\key} \def\kbdsub#1#2#3\par{% \def\one{#1}\def\three{#3}\def\threex{??}% \ifx\one\xkey\ifx\threex\three \key{#2}% \else{\tclose{\kbdfont\setupmarkupstyle{kbd}\look}}\fi \else{\tclose{\kbdfont\setupmarkupstyle{kbd}\look}}\fi } % definition of @key that produces a lozenge. Doesn't adjust to text size. %\setfont\keyrm\rmshape{8}{1000}{OT1} %\font\keysy=cmsy9 %\def\key#1{{\keyrm\textfont2=\keysy \leavevmode\hbox{% % \raise0.4pt\hbox{\angleleft}\kern-.08em\vtop{% % \vbox{\hrule\kern-0.4pt % \hbox{\raise0.4pt\hbox{\vphantom{\angleleft}}#1}}% % \kern-0.4pt\hrule}% % \kern-.06em\raise0.4pt\hbox{\angleright}}}} % definition of @key with no lozenge. If the current font is already % monospace, don't change it; that way, we respect @kbdinputstyle. But % if it isn't monospace, then use \tt. % \def\key#1{{\setupmarkupstyle{key}% \nohyphenation \ifmonospace\else\tt\fi #1}\null} % @clicksequence{File @click{} Open ...} \def\clicksequence#1{\begingroup #1\endgroup} % @clickstyle @arrow (by default) \parseargdef\clickstyle{\def\click{#1}} \def\click{\arrow} % Typeset a dimension, e.g., `in' or `pt'. The only reason for the % argument is to make the input look right: @dmn{pt} instead of @dmn{}pt. % \def\dmn#1{\thinspace #1} % @acronym for "FBI", "NATO", and the like. % We print this one point size smaller, since it's intended for % all-uppercase. % \def\acronym#1{\doacronym #1,,\finish} \def\doacronym#1,#2,#3\finish{% {\switchtolsize #1}% \def\temp{#2}% \ifx\temp\empty \else \space ({\unsepspaces \ignorespaces \temp \unskip})% \fi \null % reset \spacefactor=1000 } % @abbr for "Comput. J." and the like. % No font change, but don't do end-of-sentence spacing. % \def\abbr#1{\doabbr #1,,\finish} \def\doabbr#1,#2,#3\finish{% {\plainfrenchspacing #1}% \def\temp{#2}% \ifx\temp\empty \else \space ({\unsepspaces \ignorespaces \temp \unskip})% \fi \null % reset \spacefactor=1000 } % @asis just yields its argument. Used with @table, for example. % \def\asis#1{#1} % @math outputs its argument in math mode. % % One complication: _ usually means subscripts, but it could also mean % an actual _ character, as in @math{@var{some_variable} + 1}. So make % _ active, and distinguish by seeing if the current family is \slfam, % which is what @var uses. { \catcode`\_ = \active \gdef\mathunderscore{% \catcode`\_=\active \def_{\ifnum\fam=\slfam \_\else\sb\fi}% } } % Another complication: we want \\ (and @\) to output a math (or tt) \. % FYI, plain.tex uses \\ as a temporary control sequence (for no % particular reason), but this is not advertised and we don't care. % % The \mathchar is class=0=ordinary, family=7=ttfam, position=5C=\. \def\mathbackslash{\ifnum\fam=\ttfam \mathchar"075C \else\backslash \fi} % \def\math{% \ifmmode\else % only go into math if not in math mode already \tex \mathunderscore \let\\ = \mathbackslash \mathactive % make the texinfo accent commands work in math mode \let\"=\ddot \let\'=\acute \let\==\bar \let\^=\hat \let\`=\grave \let\u=\breve \let\v=\check \let\~=\tilde \let\dotaccent=\dot % have to provide another name for sup operator \let\mathopsup=\sup $\expandafter\finishmath\fi } \def\finishmath#1{#1$\endgroup} % Close the group opened by \tex. % Some active characters (such as <) are spaced differently in math. % We have to reset their definitions in case the @math was an argument % to a command which sets the catcodes (such as @item or @section). % { \catcode`^ = \active \catcode`< = \active \catcode`> = \active \catcode`+ = \active \catcode`' = \active \gdef\mathactive{% \let^ = \ptexhat \let< = \ptexless \let> = \ptexgtr \let+ = \ptexplus \let' = \ptexquoteright } } % for @sub and @sup, if in math mode, just do a normal sub/superscript. % If in text, use math to place as sub/superscript, but switch % into text mode, with smaller fonts. This is a different font than the % one used for real math sub/superscripts (8pt vs. 7pt), but let's not % fix it (significant additions to font machinery) until someone notices. % \def\sub{\ifmmode \expandafter\sb \else \expandafter\finishsub\fi} \def\finishsub#1{$\sb{\hbox{\switchtolllsize #1}}$}% % \def\sup{\ifmmode \expandafter\ptexsp \else \expandafter\finishsup\fi} \def\finishsup#1{$\ptexsp{\hbox{\switchtolllsize #1}}$}% % @inlinefmt{FMTNAME,PROCESSED-TEXT} and @inlineraw{FMTNAME,RAW-TEXT}. % Ignore unless FMTNAME == tex; then it is like @iftex and @tex, % except specified as a normal braced arg, so no newlines to worry about. % \def\outfmtnametex{tex} % \long\def\inlinefmt#1{\doinlinefmt #1,\finish} \long\def\doinlinefmt#1,#2,\finish{% \def\inlinefmtname{#1}% \ifx\inlinefmtname\outfmtnametex \ignorespaces #2\fi } % % @inlinefmtifelse{FMTNAME,THEN-TEXT,ELSE-TEXT} expands THEN-TEXT if % FMTNAME is tex, else ELSE-TEXT. \long\def\inlinefmtifelse#1{\doinlinefmtifelse #1,,,\finish} \long\def\doinlinefmtifelse#1,#2,#3,#4,\finish{% \def\inlinefmtname{#1}% \ifx\inlinefmtname\outfmtnametex \ignorespaces #2\else \ignorespaces #3\fi } % % For raw, must switch into @tex before parsing the argument, to avoid % setting catcodes prematurely. Doing it this way means that, for % example, @inlineraw{html, foo{bar} gets a parse error instead of being % ignored. But this isn't important because if people want a literal % *right* brace they would have to use a command anyway, so they may as % well use a command to get a left brace too. We could re-use the % delimiter character idea from \verb, but it seems like overkill. % \long\def\inlineraw{\tex \doinlineraw} \long\def\doinlineraw#1{\doinlinerawtwo #1,\finish} \def\doinlinerawtwo#1,#2,\finish{% \def\inlinerawname{#1}% \ifx\inlinerawname\outfmtnametex \ignorespaces #2\fi \endgroup % close group opened by \tex. } % @inlineifset{VAR, TEXT} expands TEXT if VAR is @set. % \long\def\inlineifset#1{\doinlineifset #1,\finish} \long\def\doinlineifset#1,#2,\finish{% \def\inlinevarname{#1}% \expandafter\ifx\csname SET\inlinevarname\endcsname\relax \else\ignorespaces#2\fi } % @inlineifclear{VAR, TEXT} expands TEXT if VAR is not @set. % \long\def\inlineifclear#1{\doinlineifclear #1,\finish} \long\def\doinlineifclear#1,#2,\finish{% \def\inlinevarname{#1}% \expandafter\ifx\csname SET\inlinevarname\endcsname\relax \ignorespaces#2\fi } \message{glyphs,} % and logos. % @@ prints an @, as does @atchar{}. \def\@{\char64 } \let\atchar=\@ % @{ @} @lbracechar{} @rbracechar{} all generate brace characters. \def\lbracechar{{\ifmonospace\char123\else\ensuremath\lbrace\fi}} \def\rbracechar{{\ifmonospace\char125\else\ensuremath\rbrace\fi}} \let\{=\lbracechar \let\}=\rbracechar % @comma{} to avoid , parsing problems. \let\comma = , % Accents: @, @dotaccent @ringaccent @ubaraccent @udotaccent % Others are defined by plain TeX: @` @' @" @^ @~ @= @u @v @H. \let\, = \ptexc \let\dotaccent = \ptexdot \def\ringaccent#1{{\accent23 #1}} \let\tieaccent = \ptext \let\ubaraccent = \ptexb \let\udotaccent = \d % Other special characters: @questiondown @exclamdown @ordf @ordm % Plain TeX defines: @AA @AE @O @OE @L (plus lowercase versions) @ss. \def\questiondown{?`} \def\exclamdown{!`} \def\ordf{\leavevmode\raise1ex\hbox{\switchtolllsize \underbar{a}}} \def\ordm{\leavevmode\raise1ex\hbox{\switchtolllsize \underbar{o}}} % Dotless i and dotless j, used for accents. \def\imacro{i} \def\jmacro{j} \def\dotless#1{% \def\temp{#1}% \ifx\temp\imacro \ifmmode\imath \else\ptexi \fi \else\ifx\temp\jmacro \ifmmode\jmath \else\j \fi \else \errmessage{@dotless can be used only with i or j}% \fi\fi } % The \TeX{} logo, as in plain, but resetting the spacing so that a % period following counts as ending a sentence. (Idea found in latex.) % \edef\TeX{\TeX \spacefactor=1000 } % @LaTeX{} logo. Not quite the same results as the definition in % latex.ltx, since we use a different font for the raised A; it's most % convenient for us to use an explicitly smaller font, rather than using % the \scriptstyle font (since we don't reset \scriptstyle and % \scriptscriptstyle). % \def\LaTeX{% L\kern-.36em {\setbox0=\hbox{T}% \vbox to \ht0{\hbox{% \ifx\textnominalsize\xwordpt % for 10pt running text, lllsize (8pt) is too small for the A in LaTeX. % Revert to plain's \scriptsize, which is 7pt. \count255=\the\fam $\fam\count255 \scriptstyle A$% \else % For 11pt, we can use our lllsize. \switchtolllsize A% \fi }% \vss }}% \kern-.15em \TeX } % Some math mode symbols. Define \ensuremath to switch into math mode % unless we are already there. Expansion tricks may not be needed here, % but safer, and can't hurt. \def\ensuremath{\ifmmode \expandafter\asis \else\expandafter\ensuredmath \fi} \def\ensuredmath#1{$\relax#1$} % \def\bullet{\ensuremath\ptexbullet} \def\geq{\ensuremath\ge} \def\leq{\ensuremath\le} \def\minus{\ensuremath-} % @dots{} outputs an ellipsis using the current font. % We do .5em per period so that it has the same spacing in the cm % typewriter fonts as three actual period characters; on the other hand, % in other typewriter fonts three periods are wider than 1.5em. So do % whichever is larger. % \def\dots{% \leavevmode \setbox0=\hbox{...}% get width of three periods \ifdim\wd0 > 1.5em \dimen0 = \wd0 \else \dimen0 = 1.5em \fi \hbox to \dimen0{% \hskip 0pt plus.25fil .\hskip 0pt plus1fil .\hskip 0pt plus1fil .\hskip 0pt plus.5fil }% } % @enddots{} is an end-of-sentence ellipsis. % \def\enddots{% \dots \spacefactor=\endofsentencespacefactor } % @point{}, @result{}, @expansion{}, @print{}, @equiv{}. % % Since these characters are used in examples, they should be an even number of % \tt widths. Each \tt character is 1en, so two makes it 1em. % \def\point{$\star$} \def\arrow{\leavevmode\raise.05ex\hbox to 1em{\hfil$\rightarrow$\hfil}} \def\result{\leavevmode\raise.05ex\hbox to 1em{\hfil$\Rightarrow$\hfil}} \def\expansion{\leavevmode\hbox to 1em{\hfil$\mapsto$\hfil}} \def\print{\leavevmode\lower.1ex\hbox to 1em{\hfil$\dashv$\hfil}} \def\equiv{\leavevmode\hbox to 1em{\hfil$\ptexequiv$\hfil}} % The @error{} command. % Adapted from the TeXbook's \boxit. % \newbox\errorbox % {\ttfont \global\dimen0 = 3em}% Width of the box. \dimen2 = .55pt % Thickness of rules % The text. (`r' is open on the right, `e' somewhat less so on the left.) \setbox0 = \hbox{\kern-.75pt \reducedsf \putworderror\kern-1.5pt} % \setbox\errorbox=\hbox to \dimen0{\hfil \hsize = \dimen0 \advance\hsize by -5.8pt % Space to left+right. \advance\hsize by -2\dimen2 % Rules. \vbox{% \hrule height\dimen2 \hbox{\vrule width\dimen2 \kern3pt % Space to left of text. \vtop{\kern2.4pt \box0 \kern2.4pt}% Space above/below. \kern3pt\vrule width\dimen2}% Space to right. \hrule height\dimen2} \hfil} % \def\error{\leavevmode\lower.7ex\copy\errorbox} % @pounds{} is a sterling sign, which Knuth put in the CM italic font. % \def\pounds{{\it\$}} % @euro{} comes from a separate font, depending on the current style. % We use the free feym* fonts from the eurosym package by Henrik % Theiling, which support regular, slanted, bold and bold slanted (and % "outlined" (blackboard board, sort of) versions, which we don't need). % It is available from http://www.ctan.org/tex-archive/fonts/eurosym. % % Although only regular is the truly official Euro symbol, we ignore % that. The Euro is designed to be slightly taller than the regular % font height. % % feymr - regular % feymo - slanted % feybr - bold % feybo - bold slanted % % There is no good (free) typewriter version, to my knowledge. % A feymr10 euro is ~7.3pt wide, while a normal cmtt10 char is ~5.25pt wide. % Hmm. % % Also doesn't work in math. Do we need to do math with euro symbols? % Hope not. % % \def\euro{{\eurofont e}} \def\eurofont{% % We set the font at each command, rather than predefining it in % \textfonts and the other font-switching commands, so that % installations which never need the symbol don't have to have the % font installed. % % There is only one designed size (nominal 10pt), so we always scale % that to the current nominal size. % % By the way, simply using "at 1em" works for cmr10 and the like, but % does not work for cmbx10 and other extended/shrunken fonts. % \def\eurosize{\csname\curfontsize nominalsize\endcsname}% % \ifx\curfontstyle\bfstylename % bold: \font\thiseurofont = \ifusingit{feybo10}{feybr10} at \eurosize \else % regular: \font\thiseurofont = \ifusingit{feymo10}{feymr10} at \eurosize \fi \thiseurofont } % Glyphs from the EC fonts. We don't use \let for the aliases, because % sometimes we redefine the original macro, and the alias should reflect % the redefinition. % % Use LaTeX names for the Icelandic letters. \def\DH{{\ecfont \char"D0}} % Eth \def\dh{{\ecfont \char"F0}} % eth \def\TH{{\ecfont \char"DE}} % Thorn \def\th{{\ecfont \char"FE}} % thorn % \def\guillemetleft{{\ecfont \char"13}} \def\guillemotleft{\guillemetleft} \def\guillemetright{{\ecfont \char"14}} \def\guillemotright{\guillemetright} \def\guilsinglleft{{\ecfont \char"0E}} \def\guilsinglright{{\ecfont \char"0F}} \def\quotedblbase{{\ecfont \char"12}} \def\quotesinglbase{{\ecfont \char"0D}} % % This positioning is not perfect (see the ogonek LaTeX package), but % we have the precomposed glyphs for the most common cases. We put the % tests to use those glyphs in the single \ogonek macro so we have fewer % dummy definitions to worry about for index entries, etc. % % ogonek is also used with other letters in Lithuanian (IOU), but using % the precomposed glyphs for those is not so easy since they aren't in % the same EC font. \def\ogonek#1{{% \def\temp{#1}% \ifx\temp\macrocharA\Aogonek \else\ifx\temp\macrochara\aogonek \else\ifx\temp\macrocharE\Eogonek \else\ifx\temp\macrochare\eogonek \else \ecfont \setbox0=\hbox{#1}% \ifdim\ht0=1ex\accent"0C #1% \else\ooalign{\unhbox0\crcr\hidewidth\char"0C \hidewidth}% \fi \fi\fi\fi\fi }% } \def\Aogonek{{\ecfont \char"81}}\def\macrocharA{A} \def\aogonek{{\ecfont \char"A1}}\def\macrochara{a} \def\Eogonek{{\ecfont \char"86}}\def\macrocharE{E} \def\eogonek{{\ecfont \char"A6}}\def\macrochare{e} % % Use the European Computer Modern fonts (cm-super in outline format) % for non-CM glyphs. That is ec* for regular text and tc* for the text % companion symbols (LaTeX TS1 encoding). Both are part of the ec % package and follow the same conventions. % \def\ecfont{\etcfont{e}} \def\tcfont{\etcfont{t}} % \def\etcfont#1{% % We can't distinguish serif/sans and italic/slanted, but this % is used for crude hacks anyway (like adding French and German % quotes to documents typeset with CM, where we lose kerning), so % hopefully nobody will notice/care. \edef\ecsize{\csname\curfontsize ecsize\endcsname}% \edef\nominalsize{\csname\curfontsize nominalsize\endcsname}% \ifmonospace % typewriter: \font\thisecfont = #1ctt\ecsize \space at \nominalsize \else \ifx\curfontstyle\bfstylename % bold: \font\thisecfont = #1cb\ifusingit{i}{x}\ecsize \space at \nominalsize \else % regular: \font\thisecfont = #1c\ifusingit{ti}{rm}\ecsize \space at \nominalsize \fi \fi \thisecfont } % @registeredsymbol - R in a circle. The font for the R should really % be smaller yet, but lllsize is the best we can do for now. % Adapted from the plain.tex definition of \copyright. % \def\registeredsymbol{% $^{{\ooalign{\hfil\raise.07ex\hbox{\switchtolllsize R}% \hfil\crcr\Orb}}% }$% } % @textdegree - the normal degrees sign. % \def\textdegree{$^\circ$} % Laurent Siebenmann reports \Orb undefined with: % Textures 1.7.7 (preloaded format=plain 93.10.14) (68K) 16 APR 2004 02:38 % so we'll define it if necessary. % \ifx\Orb\thisisundefined \def\Orb{\mathhexbox20D} \fi % Quotes. \chardef\quotedblleft="5C \chardef\quotedblright=`\" \chardef\quoteleft=`\` \chardef\quoteright=`\' \message{page headings,} \newskip\titlepagetopglue \titlepagetopglue = 1.5in \newskip\titlepagebottomglue \titlepagebottomglue = 2pc % First the title page. Must do @settitle before @titlepage. \newif\ifseenauthor \newif\iffinishedtitlepage % @setcontentsaftertitlepage used to do an implicit @contents or % @shortcontents after @end titlepage, but it is now obsolete. \def\setcontentsaftertitlepage{% \errmessage{@setcontentsaftertitlepage has been removed as a Texinfo command; move your @contents command if you want the contents after the title page.}}% \def\setshortcontentsaftertitlepage{% \errmessage{@setshortcontentsaftertitlepage has been removed as a Texinfo command; move your @shortcontents and @contents commands if you want the contents after the title page.}}% \parseargdef\shorttitlepage{% \begingroup \hbox{}\vskip 1.5in \chaprm \centerline{#1}% \endgroup\page\hbox{}\page} \envdef\titlepage{% % Open one extra group, as we want to close it in the middle of \Etitlepage. \begingroup \parindent=0pt \textfonts % Leave some space at the very top of the page. \vglue\titlepagetopglue % No rule at page bottom unless we print one at the top with @title. \finishedtitlepagetrue % % Most title ``pages'' are actually two pages long, with space % at the top of the second. We don't want the ragged left on the second. \let\oldpage = \page \def\page{% \iffinishedtitlepage\else \finishtitlepage \fi \let\page = \oldpage \page \null }% } \def\Etitlepage{% \iffinishedtitlepage\else \finishtitlepage \fi % It is important to do the page break before ending the group, % because the headline and footline are only empty inside the group. % If we use the new definition of \page, we always get a blank page % after the title page, which we certainly don't want. \oldpage \endgroup % % Need this before the \...aftertitlepage checks so that if they are % in effect the toc pages will come out with page numbers. \HEADINGSon } \def\finishtitlepage{% \vskip4pt \hrule height 2pt width \hsize \vskip\titlepagebottomglue \finishedtitlepagetrue } % Settings used for typesetting titles: no hyphenation, no indentation, % don't worry much about spacing, ragged right. This should be used % inside a \vbox, and fonts need to be set appropriately first. \par should % be specified before the end of the \vbox, since a vbox is a group. % \def\raggedtitlesettings{% \rm \hyphenpenalty=10000 \parindent=0pt \tolerance=5000 \ptexraggedright } % Macros to be used within @titlepage: \let\subtitlerm=\rmfont \def\subtitlefont{\subtitlerm \normalbaselineskip = 13pt \normalbaselines} \parseargdef\title{% \checkenv\titlepage \vbox{\titlefonts \raggedtitlesettings #1\par}% % print a rule at the page bottom also. \finishedtitlepagefalse \vskip4pt \hrule height 4pt width \hsize \vskip4pt } \parseargdef\subtitle{% \checkenv\titlepage {\subtitlefont \rightline{#1}}% } % @author should come last, but may come many times. % It can also be used inside @quotation. % \parseargdef\author{% \def\temp{\quotation}% \ifx\thisenv\temp \def\quotationauthor{#1}% printed in \Equotation. \else \checkenv\titlepage \ifseenauthor\else \vskip 0pt plus 1filll \seenauthortrue \fi {\secfonts\rm \leftline{#1}}% \fi } % Set up page headings and footings. \let\thispage=\folio \newtoks\evenheadline % headline on even pages \newtoks\oddheadline % headline on odd pages \newtoks\evenfootline % footline on even pages \newtoks\oddfootline % footline on odd pages % Now make \makeheadline and \makefootline in Plain TeX use those variables \headline={{\textfonts\rm \ifodd\pageno \the\oddheadline \else \the\evenheadline \fi}} \footline={{\textfonts\rm \ifodd\pageno \the\oddfootline \else \the\evenfootline \fi}\HEADINGShook} \let\HEADINGShook=\relax % Commands to set those variables. % For example, this is what @headings on does % @evenheading @thistitle|@thispage|@thischapter % @oddheading @thischapter|@thispage|@thistitle % @evenfooting @thisfile|| % @oddfooting ||@thisfile \def\evenheading{\parsearg\evenheadingxxx} \def\evenheadingxxx #1{\evenheadingyyy #1\|\|\|\|\finish} \def\evenheadingyyy #1\|#2\|#3\|#4\finish{% \global\evenheadline={\rlap{\centerline{#2}}\line{#1\hfil#3}}} \def\oddheading{\parsearg\oddheadingxxx} \def\oddheadingxxx #1{\oddheadingyyy #1\|\|\|\|\finish} \def\oddheadingyyy #1\|#2\|#3\|#4\finish{% \global\oddheadline={\rlap{\centerline{#2}}\line{#1\hfil#3}}} \parseargdef\everyheading{\oddheadingxxx{#1}\evenheadingxxx{#1}}% \def\evenfooting{\parsearg\evenfootingxxx} \def\evenfootingxxx #1{\evenfootingyyy #1\|\|\|\|\finish} \def\evenfootingyyy #1\|#2\|#3\|#4\finish{% \global\evenfootline={\rlap{\centerline{#2}}\line{#1\hfil#3}}} \def\oddfooting{\parsearg\oddfootingxxx} \def\oddfootingxxx #1{\oddfootingyyy #1\|\|\|\|\finish} \def\oddfootingyyy #1\|#2\|#3\|#4\finish{% \global\oddfootline = {\rlap{\centerline{#2}}\line{#1\hfil#3}}% % % Leave some space for the footline. Hopefully ok to assume % @evenfooting will not be used by itself. \global\advance\txipageheight by -12pt \global\advance\vsize by -12pt } \parseargdef\everyfooting{\oddfootingxxx{#1}\evenfootingxxx{#1}} % @evenheadingmarks top \thischapter <- chapter at the top of a page % @evenheadingmarks bottom \thischapter <- chapter at the bottom of a page % % The same set of arguments for: % % @oddheadingmarks % @evenfootingmarks % @oddfootingmarks % @everyheadingmarks % @everyfootingmarks % These define \getoddheadingmarks, \getevenheadingmarks, % \getoddfootingmarks, and \getevenfootingmarks, each to one of % \gettopheadingmarks, \getbottomheadingmarks. % \def\evenheadingmarks{\headingmarks{even}{heading}} \def\oddheadingmarks{\headingmarks{odd}{heading}} \def\evenfootingmarks{\headingmarks{even}{footing}} \def\oddfootingmarks{\headingmarks{odd}{footing}} \parseargdef\everyheadingmarks{\headingmarks{even}{heading}{#1} \headingmarks{odd}{heading}{#1} } \parseargdef\everyfootingmarks{\headingmarks{even}{footing}{#1} \headingmarks{odd}{footing}{#1} } % #1 = even/odd, #2 = heading/footing, #3 = top/bottom. \def\headingmarks#1#2#3 {% \expandafter\let\expandafter\temp \csname get#3headingmarks\endcsname \global\expandafter\let\csname get#1#2marks\endcsname \temp } \everyheadingmarks bottom \everyfootingmarks bottom % @headings double turns headings on for double-sided printing. % @headings single turns headings on for single-sided printing. % @headings off turns them off. % @headings on same as @headings double, retained for compatibility. % @headings after turns on double-sided headings after this page. % @headings doubleafter turns on double-sided headings after this page. % @headings singleafter turns on single-sided headings after this page. % By default, they are off at the start of a document, % and turned `on' after @end titlepage. \parseargdef\headings{\csname HEADINGS#1\endcsname} \def\headingsoff{% non-global headings elimination \evenheadline={\hfil}\evenfootline={\hfil}% \oddheadline={\hfil}\oddfootline={\hfil}% } \def\HEADINGSoff{{\globaldefs=1 \headingsoff}} % global setting \HEADINGSoff % it's the default % When we turn headings on, set the page number to 1. % For double-sided printing, put current file name in lower left corner, % chapter name on inside top of right hand pages, document % title on inside top of left hand pages, and page numbers on outside top % edge of all pages. \def\HEADINGSdouble{% \global\pageno=1 \global\evenfootline={\hfil} \global\oddfootline={\hfil} \global\evenheadline={\line{\folio\hfil\thistitle}} \global\oddheadline={\line{\thischapterheading\hfil\folio}} \global\let\contentsalignmacro = \chapoddpage } \let\contentsalignmacro = \chappager % For single-sided printing, chapter title goes across top left of page, % page number on top right. \def\HEADINGSsingle{% \global\pageno=1 \global\evenfootline={\hfil} \global\oddfootline={\hfil} \global\evenheadline={\line{\thischapterheading\hfil\folio}} \global\oddheadline={\line{\thischapterheading\hfil\folio}} \global\let\contentsalignmacro = \chappager } \def\HEADINGSon{\HEADINGSdouble} \def\HEADINGSafter{\let\HEADINGShook=\HEADINGSdoublex} \let\HEADINGSdoubleafter=\HEADINGSafter \def\HEADINGSdoublex{% \global\evenfootline={\hfil} \global\oddfootline={\hfil} \global\evenheadline={\line{\folio\hfil\thistitle}} \global\oddheadline={\line{\thischapterheading\hfil\folio}} \global\let\contentsalignmacro = \chapoddpage } \def\HEADINGSsingleafter{\let\HEADINGShook=\HEADINGSsinglex} \def\HEADINGSsinglex{% \global\evenfootline={\hfil} \global\oddfootline={\hfil} \global\evenheadline={\line{\thischapterheading\hfil\folio}} \global\oddheadline={\line{\thischapterheading\hfil\folio}} \global\let\contentsalignmacro = \chappager } % Subroutines used in generating headings % This produces Day Month Year style of output. % Only define if not already defined, in case a txi-??.tex file has set % up a different format (e.g., txi-cs.tex does this). \ifx\today\thisisundefined \def\today{% \number\day\space \ifcase\month \or\putwordMJan\or\putwordMFeb\or\putwordMMar\or\putwordMApr \or\putwordMMay\or\putwordMJun\or\putwordMJul\or\putwordMAug \or\putwordMSep\or\putwordMOct\or\putwordMNov\or\putwordMDec \fi \space\number\year} \fi % @settitle line... specifies the title of the document, for headings. % It generates no output of its own. \def\thistitle{\putwordNoTitle} \def\settitle{\parsearg{\gdef\thistitle}} \message{tables,} % Tables -- @table, @ftable, @vtable, @item(x). % default indentation of table text \newdimen\tableindent \tableindent=.8in % default indentation of @itemize and @enumerate text \newdimen\itemindent \itemindent=.3in % margin between end of table item and start of table text. \newdimen\itemmargin \itemmargin=.1in % used internally for \itemindent minus \itemmargin \newdimen\itemmax % Note @table, @ftable, and @vtable define @item, @itemx, etc., with % these defs. % They also define \itemindex % to index the item name in whatever manner is desired (perhaps none). \newif\ifitemxneedsnegativevskip \def\itemxpar{\par\ifitemxneedsnegativevskip\nobreak\vskip-\parskip\nobreak\fi} \def\internalBitem{\smallbreak \parsearg\itemzzz} \def\internalBitemx{\itemxpar \parsearg\itemzzz} \def\itemzzz #1{\begingroup % \advance\hsize by -\rightskip \advance\hsize by -\tableindent \setbox0=\hbox{\itemindicate{#1}}% \itemindex{#1}% \nobreak % This prevents a break before @itemx. % % If the item text does not fit in the space we have, put it on a line % by itself, and do not allow a page break either before or after that % line. We do not start a paragraph here because then if the next % command is, e.g., @kindex, the whatsit would get put into the % horizontal list on a line by itself, resulting in extra blank space. \ifdim \wd0>\itemmax % % Make this a paragraph so we get the \parskip glue and wrapping, % but leave it ragged-right. \begingroup \advance\leftskip by-\tableindent \advance\hsize by\tableindent \advance\rightskip by0pt plus1fil\relax \leavevmode\unhbox0\par \endgroup % % We're going to be starting a paragraph, but we don't want the % \parskip glue -- logically it's part of the @item we just started. \nobreak \vskip-\parskip % % Stop a page break at the \parskip glue coming up. However, if % what follows is an environment such as @example, there will be no % \parskip glue; then the negative vskip we just inserted would % cause the example and the item to crash together. So we use this % bizarre value of 10001 as a signal to \aboveenvbreak to insert % \parskip glue after all. Section titles are handled this way also. % \penalty 10001 \endgroup \itemxneedsnegativevskipfalse \else % The item text fits into the space. Start a paragraph, so that the % following text (if any) will end up on the same line. \noindent % Do this with kerns and \unhbox so that if there is a footnote in % the item text, it can migrate to the main vertical list and % eventually be printed. \nobreak\kern-\tableindent \dimen0 = \itemmax \advance\dimen0 by \itemmargin \advance\dimen0 by -\wd0 \unhbox0 \nobreak\kern\dimen0 \endgroup \itemxneedsnegativevskiptrue \fi } \def\item{\errmessage{@item while not in a list environment}} \def\itemx{\errmessage{@itemx while not in a list environment}} % @table, @ftable, @vtable. \envdef\table{% \let\itemindex\gobble \tablecheck{table}% } \envdef\ftable{% \def\itemindex ##1{\doind {fn}{\code{##1}}}% \tablecheck{ftable}% } \envdef\vtable{% \def\itemindex ##1{\doind {vr}{\code{##1}}}% \tablecheck{vtable}% } \def\tablecheck#1{% \ifnum \the\catcode`\^^M=\active \endgroup \errmessage{This command won't work in this context; perhaps the problem is that we are \inenvironment\thisenv}% \def\next{\doignore{#1}}% \else \let\next\tablex \fi \next } \def\tablex#1{% \def\itemindicate{#1}% \parsearg\tabley } \def\tabley#1{% {% \makevalueexpandable \edef\temp{\noexpand\tablez #1\space\space\space}% \expandafter }\temp \endtablez } \def\tablez #1 #2 #3 #4\endtablez{% \aboveenvbreak \ifnum 0#1>0 \advance \leftskip by #1\mil \fi \ifnum 0#2>0 \tableindent=#2\mil \fi \ifnum 0#3>0 \advance \rightskip by #3\mil \fi \itemmax=\tableindent \advance \itemmax by -\itemmargin \advance \leftskip by \tableindent \exdentamount=\tableindent \parindent = 0pt \parskip = \smallskipamount \ifdim \parskip=0pt \parskip=2pt \fi \let\item = \internalBitem \let\itemx = \internalBitemx } \def\Etable{\endgraf\afterenvbreak} \let\Eftable\Etable \let\Evtable\Etable \let\Eitemize\Etable \let\Eenumerate\Etable % This is the counter used by @enumerate, which is really @itemize \newcount \itemno \envdef\itemize{\parsearg\doitemize} \def\doitemize#1{% \aboveenvbreak \itemmax=\itemindent \advance\itemmax by -\itemmargin \advance\leftskip by \itemindent \exdentamount=\itemindent \parindent=0pt \parskip=\smallskipamount \ifdim\parskip=0pt \parskip=2pt \fi % % Try typesetting the item mark so that if the document erroneously says % something like @itemize @samp (intending @table), there's an error % right away at the @itemize. It's not the best error message in the % world, but it's better than leaving it to the @item. This means if % the user wants an empty mark, they have to say @w{} not just @w. \def\itemcontents{#1}% \setbox0 = \hbox{\itemcontents}% % % @itemize with no arg is equivalent to @itemize @bullet. \ifx\itemcontents\empty\def\itemcontents{\bullet}\fi % \let\item=\itemizeitem } % Definition of @item while inside @itemize and @enumerate. % \def\itemizeitem{% \advance\itemno by 1 % for enumerations {\let\par=\endgraf \smallbreak}% reasonable place to break {% % If the document has an @itemize directly after a section title, a % \nobreak will be last on the list, and \sectionheading will have % done a \vskip-\parskip. In that case, we don't want to zero % parskip, or the item text will crash with the heading. On the % other hand, when there is normal text preceding the item (as there % usually is), we do want to zero parskip, or there would be too much % space. In that case, we won't have a \nobreak before. At least % that's the theory. \ifnum\lastpenalty<10000 \parskip=0in \fi \noindent \hbox to 0pt{\hss \itemcontents \kern\itemmargin}% % \ifinner\else \vadjust{\penalty 1200}% not good to break after first line of item. \fi % We can be in inner vertical mode in a footnote, although an % @itemize looks awful there. }% \flushcr } % \splitoff TOKENS\endmark defines \first to be the first token in % TOKENS, and \rest to be the remainder. % \def\splitoff#1#2\endmark{\def\first{#1}\def\rest{#2}}% % Allow an optional argument of an uppercase letter, lowercase letter, % or number, to specify the first label in the enumerated list. No % argument is the same as `1'. % \envparseargdef\enumerate{\enumeratey #1 \endenumeratey} \def\enumeratey #1 #2\endenumeratey{% % If we were given no argument, pretend we were given `1'. \def\thearg{#1}% \ifx\thearg\empty \def\thearg{1}\fi % % Detect if the argument is a single token. If so, it might be a % letter. Otherwise, the only valid thing it can be is a number. % (We will always have one token, because of the test we just made. % This is a good thing, since \splitoff doesn't work given nothing at % all -- the first parameter is undelimited.) \expandafter\splitoff\thearg\endmark \ifx\rest\empty % Only one token in the argument. It could still be anything. % A ``lowercase letter'' is one whose \lccode is nonzero. % An ``uppercase letter'' is one whose \lccode is both nonzero, and % not equal to itself. % Otherwise, we assume it's a number. % % We need the \relax at the end of the \ifnum lines to stop TeX from % continuing to look for a <number>. % \ifnum\lccode\expandafter`\thearg=0\relax \numericenumerate % a number (we hope) \else % It's a letter. \ifnum\lccode\expandafter`\thearg=\expandafter`\thearg\relax \lowercaseenumerate % lowercase letter \else \uppercaseenumerate % uppercase letter \fi \fi \else % Multiple tokens in the argument. We hope it's a number. \numericenumerate \fi } % An @enumerate whose labels are integers. The starting integer is % given in \thearg. % \def\numericenumerate{% \itemno = \thearg \startenumeration{\the\itemno}% } % The starting (lowercase) letter is in \thearg. \def\lowercaseenumerate{% \itemno = \expandafter`\thearg \startenumeration{% % Be sure we're not beyond the end of the alphabet. \ifnum\itemno=0 \errmessage{No more lowercase letters in @enumerate; get a bigger alphabet}% \fi \char\lccode\itemno }% } % The starting (uppercase) letter is in \thearg. \def\uppercaseenumerate{% \itemno = \expandafter`\thearg \startenumeration{% % Be sure we're not beyond the end of the alphabet. \ifnum\itemno=0 \errmessage{No more uppercase letters in @enumerate; get a bigger alphabet} \fi \char\uccode\itemno }% } % Call \doitemize, adding a period to the first argument and supplying the % common last two arguments. Also subtract one from the initial value in % \itemno, since @item increments \itemno. % \def\startenumeration#1{% \advance\itemno by -1 \doitemize{#1.}\flushcr } % @alphaenumerate and @capsenumerate are abbreviations for giving an arg % to @enumerate. % \def\alphaenumerate{\enumerate{a}} \def\capsenumerate{\enumerate{A}} \def\Ealphaenumerate{\Eenumerate} \def\Ecapsenumerate{\Eenumerate} % @multitable macros % Amy Hendrickson, 8/18/94, 3/6/96 % % @multitable ... @end multitable will make as many columns as desired. % Contents of each column will wrap at width given in preamble. Width % can be specified either with sample text given in a template line, % or in percent of \hsize, the current width of text on page. % Table can continue over pages but will only break between lines. % To make preamble: % % Either define widths of columns in terms of percent of \hsize: % @multitable @columnfractions .25 .3 .45 % @item ... % % Numbers following @columnfractions are the percent of the total % current hsize to be used for each column. You may use as many % columns as desired. % Or use a template: % @multitable {Column 1 template} {Column 2 template} {Column 3 template} % @item ... % using the widest term desired in each column. % Each new table line starts with @item, each subsequent new column % starts with @tab. Empty columns may be produced by supplying @tab's % with nothing between them for as many times as empty columns are needed, % ie, @tab@tab@tab will produce two empty columns. % @item, @tab do not need to be on their own lines, but it will not hurt % if they are. % Sample multitable: % @multitable {Column 1 template} {Column 2 template} {Column 3 template} % @item first col stuff @tab second col stuff @tab third col % @item % first col stuff % @tab % second col stuff % @tab % third col % @item first col stuff @tab second col stuff % @tab Many paragraphs of text may be used in any column. % % They will wrap at the width determined by the template. % @item@tab@tab This will be in third column. % @end multitable % Default dimensions may be reset by user. % @multitableparskip is vertical space between paragraphs in table. % @multitableparindent is paragraph indent in table. % @multitablecolmargin is horizontal space to be left between columns. % @multitablelinespace is space to leave between table items, baseline % to baseline. % 0pt means it depends on current normal line spacing. % \newskip\multitableparskip \newskip\multitableparindent \newdimen\multitablecolspace \newskip\multitablelinespace \multitableparskip=0pt \multitableparindent=6pt \multitablecolspace=12pt \multitablelinespace=0pt % Macros used to set up halign preamble: % \let\endsetuptable\relax \def\xendsetuptable{\endsetuptable} \let\columnfractions\relax \def\xcolumnfractions{\columnfractions} \newif\ifsetpercent % #1 is the @columnfraction, usually a decimal number like .5, but might % be just 1. We just use it, whatever it is. % \def\pickupwholefraction#1 {% \global\advance\colcount by 1 \expandafter\xdef\csname col\the\colcount\endcsname{#1\hsize}% \setuptable } \newcount\colcount \def\setuptable#1{% \def\firstarg{#1}% \ifx\firstarg\xendsetuptable \let\go = \relax \else \ifx\firstarg\xcolumnfractions \global\setpercenttrue \else \ifsetpercent \let\go\pickupwholefraction \else \global\advance\colcount by 1 \setbox0=\hbox{#1\unskip\space}% Add a normal word space as a % separator; typically that is always in the input, anyway. \expandafter\xdef\csname col\the\colcount\endcsname{\the\wd0}% \fi \fi \ifx\go\pickupwholefraction % Put the argument back for the \pickupwholefraction call, so % we'll always have a period there to be parsed. \def\go{\pickupwholefraction#1}% \else \let\go = \setuptable \fi% \fi \go } % multitable-only commands. % % @headitem starts a heading row, which we typeset in bold. Assignments % have to be global since we are inside the implicit group of an % alignment entry. \everycr below resets \everytab so we don't have to % undo it ourselves. \def\headitemfont{\b}% for people to use in the template row; not changeable \def\headitem{% \checkenv\multitable \crcr \gdef\headitemcrhook{\nobreak}% attempt to avoid page break after headings \global\everytab={\bf}% can't use \headitemfont since the parsing differs \the\everytab % for the first item }% % % default for tables with no headings. \let\headitemcrhook=\relax % % A \tab used to include \hskip1sp. But then the space in a template % line is not enough. That is bad. So let's go back to just `&' until % we again encounter the problem the 1sp was intended to solve. % --karl, nathan@acm.org, 20apr99. \def\tab{\checkenv\multitable &\the\everytab}% % @multitable ... @end multitable definitions: % \newtoks\everytab % insert after every tab. % \envdef\multitable{% \vskip\parskip \startsavinginserts % % @item within a multitable starts a normal row. % We use \def instead of \let so that if one of the multitable entries % contains an @itemize, we don't choke on the \item (seen as \crcr aka % \endtemplate) expanding \doitemize. \def\item{\crcr}% % \tolerance=9500 \hbadness=9500 \setmultitablespacing \parskip=\multitableparskip \parindent=\multitableparindent \overfullrule=0pt \global\colcount=0 % \everycr = {% \noalign{% \global\everytab={}% Reset from possible headitem. \global\colcount=0 % Reset the column counter. % % Check for saved footnotes, etc.: \checkinserts % % Perhaps a \nobreak, then reset: \headitemcrhook \global\let\headitemcrhook=\relax }% }% % \parsearg\domultitable } \def\domultitable#1{% % To parse everything between @multitable and @item: \setuptable#1 \endsetuptable % % This preamble sets up a generic column definition, which will % be used as many times as user calls for columns. % \vtop will set a single line and will also let text wrap and % continue for many paragraphs if desired. \halign\bgroup &% \global\advance\colcount by 1 \multistrut \vtop{% % Use the current \colcount to find the correct column width: \hsize=\expandafter\csname col\the\colcount\endcsname % % In order to keep entries from bumping into each other % we will add a \leftskip of \multitablecolspace to all columns after % the first one. % % If a template has been used, we will add \multitablecolspace % to the width of each template entry. % % If the user has set preamble in terms of percent of \hsize we will % use that dimension as the width of the column, and the \leftskip % will keep entries from bumping into each other. Table will start at % left margin and final column will justify at right margin. % % Make sure we don't inherit \rightskip from the outer environment. \rightskip=0pt \ifnum\colcount=1 % The first column will be indented with the surrounding text. \advance\hsize by\leftskip \else \ifsetpercent \else % If user has not set preamble in terms of percent of \hsize % we will advance \hsize by \multitablecolspace. \advance\hsize by \multitablecolspace \fi % In either case we will make \leftskip=\multitablecolspace: \leftskip=\multitablecolspace \fi % Ignoring space at the beginning and end avoids an occasional spurious % blank line, when TeX decides to break the line at the space before the % box from the multistrut, so the strut ends up on a line by itself. % For example: % @multitable @columnfractions .11 .89 % @item @code{#} % @tab Legal holiday which is valid in major parts of the whole country. % Is automatically provided with highlighting sequences respectively % marking characters. \noindent\ignorespaces##\unskip\multistrut }\cr } \def\Emultitable{% \crcr \egroup % end the \halign \global\setpercentfalse } \def\setmultitablespacing{% \def\multistrut{\strut}% just use the standard line spacing % % Compute \multitablelinespace (if not defined by user) for use in % \multitableparskip calculation. We used define \multistrut based on % this, but (ironically) that caused the spacing to be off. % See bug-texinfo report from Werner Lemberg, 31 Oct 2004 12:52:20 +0100. \ifdim\multitablelinespace=0pt \setbox0=\vbox{X}\global\multitablelinespace=\the\baselineskip \global\advance\multitablelinespace by-\ht0 \fi % Test to see if parskip is larger than space between lines of % table. If not, do nothing. % If so, set to same dimension as multitablelinespace. \ifdim\multitableparskip>\multitablelinespace \global\multitableparskip=\multitablelinespace \global\advance\multitableparskip-7pt % to keep parskip somewhat smaller % than skip between lines in the table. \fi% \ifdim\multitableparskip=0pt \global\multitableparskip=\multitablelinespace \global\advance\multitableparskip-7pt % to keep parskip somewhat smaller % than skip between lines in the table. \fi} \message{conditionals,} % @iftex, @ifnotdocbook, @ifnothtml, @ifnotinfo, @ifnotplaintext, % @ifnotxml always succeed. They currently do nothing; we don't % attempt to check whether the conditionals are properly nested. But we % have to remember that they are conditionals, so that @end doesn't % attempt to close an environment group. % \def\makecond#1{% \expandafter\let\csname #1\endcsname = \relax \expandafter\let\csname iscond.#1\endcsname = 1 } \makecond{iftex} \makecond{ifnotdocbook} \makecond{ifnothtml} \makecond{ifnotinfo} \makecond{ifnotplaintext} \makecond{ifnotxml} % Ignore @ignore, @ifhtml, @ifinfo, and the like. % \def\direntry{\doignore{direntry}} \def\documentdescription{\doignore{documentdescription}} \def\docbook{\doignore{docbook}} \def\html{\doignore{html}} \def\ifdocbook{\doignore{ifdocbook}} \def\ifhtml{\doignore{ifhtml}} \def\ifinfo{\doignore{ifinfo}} \def\ifnottex{\doignore{ifnottex}} \def\ifplaintext{\doignore{ifplaintext}} \def\ifxml{\doignore{ifxml}} \def\ignore{\doignore{ignore}} \def\menu{\doignore{menu}} \def\xml{\doignore{xml}} % Ignore text until a line `@end #1', keeping track of nested conditionals. % % A count to remember the depth of nesting. \newcount\doignorecount \def\doignore#1{\begingroup % Scan in ``verbatim'' mode: \obeylines \catcode`\@ = \other \catcode`\{ = \other \catcode`\} = \other % % Make sure that spaces turn into tokens that match what \doignoretext wants. \spaceisspace % % Count number of #1's that we've seen. \doignorecount = 0 % % Swallow text until we reach the matching `@end #1'. \dodoignore{#1}% } { \catcode`_=11 % We want to use \_STOP_ which cannot appear in texinfo source. \obeylines % % \gdef\dodoignore#1{% % #1 contains the command name as a string, e.g., `ifinfo'. % % Define a command to find the next `@end #1'. \long\def\doignoretext##1^^M@end #1{% \doignoretextyyy##1^^M@#1\_STOP_}% % % And this command to find another #1 command, at the beginning of a % line. (Otherwise, we would consider a line `@c @ifset', for % example, to count as an @ifset for nesting.) \long\def\doignoretextyyy##1^^M@#1##2\_STOP_{\doignoreyyy{##2}\_STOP_}% % % And now expand that command. \doignoretext ^^M% }% } \def\doignoreyyy#1{% \def\temp{#1}% \ifx\temp\empty % Nothing found. \let\next\doignoretextzzz \else % Found a nested condition, ... \advance\doignorecount by 1 \let\next\doignoretextyyy % ..., look for another. % If we're here, #1 ends with ^^M\ifinfo (for example). \fi \next #1% the token \_STOP_ is present just after this macro. } % We have to swallow the remaining "\_STOP_". % \def\doignoretextzzz#1{% \ifnum\doignorecount = 0 % We have just found the outermost @end. \let\next\enddoignore \else % Still inside a nested condition. \advance\doignorecount by -1 \let\next\doignoretext % Look for the next @end. \fi \next } % Finish off ignored text. { \obeylines% % Ignore anything after the last `@end #1'; this matters in verbatim % environments, where otherwise the newline after an ignored conditional % would result in a blank line in the output. \gdef\enddoignore#1^^M{\endgroup\ignorespaces}% } % @set VAR sets the variable VAR to an empty value. % @set VAR REST-OF-LINE sets VAR to the value REST-OF-LINE. % % Since we want to separate VAR from REST-OF-LINE (which might be % empty), we can't just use \parsearg; we have to insert a space of our % own to delimit the rest of the line, and then take it out again if we % didn't need it. % We rely on the fact that \parsearg sets \catcode`\ =10. % \parseargdef\set{\setyyy#1 \endsetyyy} \def\setyyy#1 #2\endsetyyy{% {% \makevalueexpandable \def\temp{#2}% \edef\next{\gdef\makecsname{SET#1}}% \ifx\temp\empty \next{}% \else \setzzz#2\endsetzzz \fi }% } % Remove the trailing space \setxxx inserted. \def\setzzz#1 \endsetzzz{\next{#1}} % @clear VAR clears (i.e., unsets) the variable VAR. % \parseargdef\clear{% {% \makevalueexpandable \global\expandafter\let\csname SET#1\endcsname=\relax }% } % @value{foo} gets the text saved in variable foo. \def\value{\begingroup\makevalueexpandable\valuexxx} \def\valuexxx#1{\expandablevalue{#1}\endgroup} { \catcode`\-=\active \catcode`\_=\active % \gdef\makevalueexpandable{% \let\value = \expandablevalue % We don't want these characters active, ... \catcode`\-=\other \catcode`\_=\other % ..., but we might end up with active ones in the argument if % we're called from @code, as @code{@value{foo-bar_}}, though. % So \let them to their normal equivalents. \let-\normaldash \let_\normalunderscore } } % We have this subroutine so that we can handle at least some @value's % properly in indexes (we call \makevalueexpandable in \indexdummies). % The command has to be fully expandable (if the variable is set), since % the result winds up in the index file. This means that if the % variable's value contains other Texinfo commands, it's almost certain % it will fail (although perhaps we could fix that with sufficient work % to do a one-level expansion on the result, instead of complete). % % Unfortunately, this has the consequence that when _ is in the *value* % of an @set, it does not print properly in the roman fonts (get the cmr % dot accent at position 126 instead). No fix comes to mind, and it's % been this way since 2003 or earlier, so just ignore it. % \def\expandablevalue#1{% \expandafter\ifx\csname SET#1\endcsname\relax {[No value for ``#1'']}% \message{Variable `#1', used in @value, is not set.}% \else \csname SET#1\endcsname \fi } % Like \expandablevalue, but completely expandable (the \message in the % definition above operates at the execution level of TeX). Used when % writing to auxiliary files, due to the expansion that \write does. % If flag is undefined, pass through an unexpanded @value command: maybe it % will be set by the time it is read back in. % % NB flag names containing - or _ may not work here. \def\dummyvalue#1{% \expandafter\ifx\csname SET#1\endcsname\relax \noexpand\value{#1}% \else \csname SET#1\endcsname \fi } % Used for @value's in index entries to form the sort key: expand the @value % if possible, otherwise sort late. \def\indexnofontsvalue#1{% \expandafter\ifx\csname SET#1\endcsname\relax ZZZZZZZ \else \csname SET#1\endcsname \fi } % @ifset VAR ... @end ifset reads the `...' iff VAR has been defined % with @set. % % To get the special treatment we need for `@end ifset,' we call % \makecond and then redefine. % \makecond{ifset} \def\ifset{\parsearg{\doifset{\let\next=\ifsetfail}}} \def\doifset#1#2{% {% \makevalueexpandable \let\next=\empty \expandafter\ifx\csname SET#2\endcsname\relax #1% If not set, redefine \next. \fi \expandafter }\next } \def\ifsetfail{\doignore{ifset}} % @ifclear VAR ... @end executes the `...' iff VAR has never been % defined with @set, or has been undefined with @clear. % % The `\else' inside the `\doifset' parameter is a trick to reuse the % above code: if the variable is not set, do nothing, if it is set, % then redefine \next to \ifclearfail. % \makecond{ifclear} \def\ifclear{\parsearg{\doifset{\else \let\next=\ifclearfail}}} \def\ifclearfail{\doignore{ifclear}} % @ifcommandisdefined CMD ... @end executes the `...' if CMD (written % without the @) is in fact defined. We can only feasibly check at the % TeX level, so something like `mathcode' is going to considered % defined even though it is not a Texinfo command. % \makecond{ifcommanddefined} \def\ifcommanddefined{\parsearg{\doifcmddefined{\let\next=\ifcmddefinedfail}}} % \def\doifcmddefined#1#2{{% \makevalueexpandable \let\next=\empty \expandafter\ifx\csname #2\endcsname\relax #1% If not defined, \let\next as above. \fi \expandafter }\next } \def\ifcmddefinedfail{\doignore{ifcommanddefined}} % @ifcommandnotdefined CMD ... handled similar to @ifclear above. \makecond{ifcommandnotdefined} \def\ifcommandnotdefined{% \parsearg{\doifcmddefined{\else \let\next=\ifcmdnotdefinedfail}}} \def\ifcmdnotdefinedfail{\doignore{ifcommandnotdefined}} % Set the `txicommandconditionals' variable, so documents have a way to % test if the @ifcommand...defined conditionals are available. \set txicommandconditionals % @dircategory CATEGORY -- specify a category of the dir file % which this file should belong to. Ignore this in TeX. \let\dircategory=\comment % @defininfoenclose. \let\definfoenclose=\comment \message{indexing,} % Index generation facilities % Define \newwrite to be identical to plain tex's \newwrite % except not \outer, so it can be used within macros and \if's. \edef\newwrite{\makecsname{ptexnewwrite}} % \newindex {foo} defines an index named IX. % It automatically defines \IXindex such that % \IXindex ...rest of line... puts an entry in the index IX. % It also defines \IXindfile to be the number of the output channel for % the file that accumulates this index. The file's extension is IX. % The name of an index should be no more than 2 characters long % for the sake of vms. % \def\newindex#1{% \expandafter\chardef\csname#1indfile\endcsname=0 \expandafter\xdef\csname#1index\endcsname{% % Define @#1index \noexpand\doindex{#1}} } % @defindex foo == \newindex{foo} % \def\defindex{\parsearg\newindex} % Define @defcodeindex, like @defindex except put all entries in @code. % \def\defcodeindex{\parsearg\newcodeindex} % \def\newcodeindex#1{% \expandafter\chardef\csname#1indfile\endcsname=0 \expandafter\xdef\csname#1index\endcsname{% \noexpand\docodeindex{#1}}% } % The default indices: \newindex{cp}% concepts, \newcodeindex{fn}% functions, \newcodeindex{vr}% variables, \newcodeindex{tp}% types, \newcodeindex{ky}% keys \newcodeindex{pg}% and programs. % @synindex foo bar makes index foo feed into index bar. % Do this instead of @defindex foo if you don't want it as a separate index. % % @syncodeindex foo bar similar, but put all entries made for index foo % inside @code. % \def\synindex#1 #2 {\dosynindex\doindex{#1}{#2}} \def\syncodeindex#1 #2 {\dosynindex\docodeindex{#1}{#2}} % #1 is \doindex or \docodeindex, #2 the index getting redefined (foo), % #3 the target index (bar). \def\dosynindex#1#2#3{% \requireopenindexfile{#3}% % redefine \fooindfile: \expandafter\let\expandafter\temp\expandafter=\csname#3indfile\endcsname \expandafter\let\csname#2indfile\endcsname=\temp % redefine \fooindex: \expandafter\xdef\csname#2index\endcsname{\noexpand#1{#3}}% } % Define \doindex, the driver for all index macros. % Argument #1 is generated by the calling \fooindex macro, % and it is the two-letter name of the index. \def\doindex#1{\edef\indexname{#1}\parsearg\doindexxxx} \def\doindexxxx #1{\doind{\indexname}{#1}} % like the previous two, but they put @code around the argument. \def\docodeindex#1{\edef\indexname{#1}\parsearg\docodeindexxxx} \def\docodeindexxxx #1{\doind{\indexname}{\code{#1}}} % Used when writing an index entry out to an index file to prevent % expansion of Texinfo commands that can appear in an index entry. % \def\indexdummies{% \escapechar = `\\ % use backslash in output files. \definedummyletter\@% \definedummyletter\ % % % For texindex which always views { and } as separators. \def\{{\lbracechar{}}% \def\}{\rbracechar{}}% % % Do the redefinitions. \definedummies } % Used for the aux and toc files, where @ is the escape character. % \def\atdummies{% \definedummyletter\@% \definedummyletter\ % \definedummyletter\{% \definedummyletter\}% % % Do the redefinitions. \definedummies \otherbackslash } % \definedummyword defines \#1 as \string\#1\space, thus effectively % preventing its expansion. This is used only for control words, % not control letters, because the \space would be incorrect for % control characters, but is needed to separate the control word % from whatever follows. % % These can be used both for control words that take an argument and % those that do not. If it is followed by {arg} in the input, then % that will dutifully get written to the index (or wherever). % % For control letters, we have \definedummyletter, which omits the % space. % \def\definedummyword #1{\def#1{\string#1\space}}% \def\definedummyletter#1{\def#1{\string#1}}% \let\definedummyaccent\definedummyletter % Called from \indexdummies and \atdummies, to effectively prevent % the expansion of commands. % \def\definedummies{% % \let\commondummyword\definedummyword \let\commondummyletter\definedummyletter \let\commondummyaccent\definedummyaccent \commondummiesnofonts % \definedummyletter\_% \definedummyletter\-% % % Non-English letters. \definedummyword\AA \definedummyword\AE \definedummyword\DH \definedummyword\L \definedummyword\O \definedummyword\OE \definedummyword\TH \definedummyword\aa \definedummyword\ae \definedummyword\dh \definedummyword\exclamdown \definedummyword\l \definedummyword\o \definedummyword\oe \definedummyword\ordf \definedummyword\ordm \definedummyword\questiondown \definedummyword\ss \definedummyword\th % % Although these internal commands shouldn't show up, sometimes they do. \definedummyword\bf \definedummyword\gtr \definedummyword\hat \definedummyword\less \definedummyword\sf \definedummyword\sl \definedummyword\tclose \definedummyword\tt % \definedummyword\LaTeX \definedummyword\TeX % % Assorted special characters. \definedummyword\atchar \definedummyword\arrow \definedummyword\bullet \definedummyword\comma \definedummyword\copyright \definedummyword\registeredsymbol \definedummyword\dots \definedummyword\enddots \definedummyword\entrybreak \definedummyword\equiv \definedummyword\error \definedummyword\euro \definedummyword\expansion \definedummyword\geq \definedummyword\guillemetleft \definedummyword\guillemetright \definedummyword\guilsinglleft \definedummyword\guilsinglright \definedummyword\lbracechar \definedummyword\leq \definedummyword\mathopsup \definedummyword\minus \definedummyword\ogonek \definedummyword\pounds \definedummyword\point \definedummyword\print \definedummyword\quotedblbase \definedummyword\quotedblleft \definedummyword\quotedblright \definedummyword\quoteleft \definedummyword\quoteright \definedummyword\quotesinglbase \definedummyword\rbracechar \definedummyword\result \definedummyword\sub \definedummyword\sup \definedummyword\textdegree % % We want to disable all macros so that they are not expanded by \write. \macrolist \let\value\dummyvalue % \normalturnoffactive } % \commondummiesnofonts: common to \definedummies and \indexnofonts. % Define \commondummyletter, \commondummyaccent and \commondummyword before % using. Used for accents, font commands, and various control letters. % \def\commondummiesnofonts{% % Control letters and accents. \commondummyletter\!% \commondummyaccent\"% \commondummyaccent\'% \commondummyletter\*% \commondummyaccent\,% \commondummyletter\.% \commondummyletter\/% \commondummyletter\:% \commondummyaccent\=% \commondummyletter\?% \commondummyaccent\^% \commondummyaccent\`% \commondummyaccent\~% \commondummyword\u \commondummyword\v \commondummyword\H \commondummyword\dotaccent \commondummyword\ogonek \commondummyword\ringaccent \commondummyword\tieaccent \commondummyword\ubaraccent \commondummyword\udotaccent \commondummyword\dotless % % Texinfo font commands. \commondummyword\b \commondummyword\i \commondummyword\r \commondummyword\sansserif \commondummyword\sc \commondummyword\slanted \commondummyword\t % % Commands that take arguments. \commondummyword\abbr \commondummyword\acronym \commondummyword\anchor \commondummyword\cite \commondummyword\code \commondummyword\command \commondummyword\dfn \commondummyword\dmn \commondummyword\email \commondummyword\emph \commondummyword\env \commondummyword\file \commondummyword\image \commondummyword\indicateurl \commondummyword\inforef \commondummyword\kbd \commondummyword\key \commondummyword\math \commondummyword\option \commondummyword\pxref \commondummyword\ref \commondummyword\samp \commondummyword\strong \commondummyword\tie \commondummyword\U \commondummyword\uref \commondummyword\url \commondummyword\var \commondummyword\verb \commondummyword\w \commondummyword\xref } % For testing: output @{ and @} in index sort strings as \{ and \}. \newif\ifusebracesinindexes \let\indexlbrace\relax \let\indexrbrace\relax {\catcode`\@=0 \catcode`\\=13 @gdef@backslashdisappear{@def\{}} } { \catcode`\<=13 \catcode`\-=13 \catcode`\`=13 \gdef\indexnonalnumdisappear{% \expandafter\ifx\csname SETtxiindexlquoteignore\endcsname\relax\else % @set txiindexlquoteignore makes us ignore left quotes in the sort term. % (Introduced for FSFS 2nd ed.) \let`=\empty \fi % \expandafter\ifx\csname SETtxiindexbackslashignore\endcsname\relax\else \backslashdisappear \fi % \expandafter\ifx\csname SETtxiindexhyphenignore\endcsname\relax\else \def-{}% \fi \expandafter\ifx\csname SETtxiindexlessthanignore\endcsname\relax\else \def<{}% \fi \expandafter\ifx\csname SETtxiindexatsignignore\endcsname\relax\else \def\@{}% \fi } \gdef\indexnonalnumreappear{% \useindexbackslash \let-\normaldash \let<\normalless \def\@{@}% } } % \indexnofonts is used when outputting the strings to sort the index % by, and when constructing control sequence names. It eliminates all % control sequences and just writes whatever the best ASCII sort string % would be for a given command (usually its argument). % \def\indexnofonts{% % Accent commands should become @asis. \def\commondummyaccent##1{\let##1\asis}% % We can just ignore other control letters. \def\commondummyletter##1{\let##1\empty}% % All control words become @asis by default; overrides below. \let\commondummyword\commondummyaccent \commondummiesnofonts % % Don't no-op \tt, since it isn't a user-level command % and is used in the definitions of the active chars like <, >, |, etc. % Likewise with the other plain tex font commands. %\let\tt=\asis % \def\ { }% \def\@{@}% \def\_{\normalunderscore}% \def\-{}% @- shouldn't affect sorting % \uccode`\1=`\{ \uppercase{\def\{{1}}% \uccode`\1=`\} \uppercase{\def\}{1}}% \let\lbracechar\{% \let\rbracechar\}% % % Non-English letters. \def\AA{AA}% \def\AE{AE}% \def\DH{DZZ}% \def\L{L}% \def\OE{OE}% \def\O{O}% \def\TH{TH}% \def\aa{aa}% \def\ae{ae}% \def\dh{dzz}% \def\exclamdown{!}% \def\l{l}% \def\oe{oe}% \def\ordf{a}% \def\ordm{o}% \def\o{o}% \def\questiondown{?}% \def\ss{ss}% \def\th{th}% % \def\LaTeX{LaTeX}% \def\TeX{TeX}% % % Assorted special characters. \defglyph gives the control sequence a % definition that removes the {} that follows its use. \defglyph\atchar{@}% \defglyph\arrow{->}% \defglyph\bullet{bullet}% \defglyph\comma{,}% \defglyph\copyright{copyright}% \defglyph\dots{...}% \defglyph\enddots{...}% \defglyph\equiv{==}% \defglyph\error{error}% \defglyph\euro{euro}% \defglyph\expansion{==>}% \defglyph\geq{>=}% \defglyph\guillemetleft{<<}% \defglyph\guillemetright{>>}% \defglyph\guilsinglleft{<}% \defglyph\guilsinglright{>}% \defglyph\leq{<=}% \defglyph\lbracechar{\{}% \defglyph\minus{-}% \defglyph\point{.}% \defglyph\pounds{pounds}% \defglyph\print{-|}% \defglyph\quotedblbase{"}% \defglyph\quotedblleft{"}% \defglyph\quotedblright{"}% \defglyph\quoteleft{`}% \defglyph\quoteright{'}% \defglyph\quotesinglbase{,}% \defglyph\rbracechar{\}}% \defglyph\registeredsymbol{R}% \defglyph\result{=>}% \defglyph\textdegree{o}% % % We need to get rid of all macros, leaving only the arguments (if present). % Of course this is not nearly correct, but it is the best we can do for now. % makeinfo does not expand macros in the argument to @deffn, which ends up % writing an index entry, and texindex isn't prepared for an index sort entry % that starts with \. % % Since macro invocations are followed by braces, we can just redefine them % to take a single TeX argument. The case of a macro invocation that % goes to end-of-line is not handled. % \macrolist \let\value\indexnofontsvalue } \def\defglyph#1#2{\def#1##1{#2}} % see above \let\SETmarginindex=\relax % put index entries in margin (undocumented)? % Most index entries go through here, but \dosubind is the general case. % #1 is the index name, #2 is the entry text. \def\doind#1#2{\dosubind{#1}{#2}{}} % There is also \dosubind {index}{topic}{subtopic} % which makes an entry in a two-level index such as the operation index. % TODO: Two-level index? Operation index? % Workhorse for all indexes. % #1 is name of index, #2 is stuff to put there, #3 is subentry -- % empty if called from \doind, as we usually are (the main exception % is with most defuns, which call us directly). % \def\dosubind#1#2#3{% \iflinks {% \requireopenindexfile{#1}% % Store the main index entry text (including the third arg). \toks0 = {#2}% % If third arg is present, precede it with a space. \def\thirdarg{#3}% \ifx\thirdarg\empty \else \toks0 = \expandafter{\the\toks0 \space #3}% \fi % \edef\writeto{\csname#1indfile\endcsname}% % \safewhatsit\dosubindwrite }% \fi } % Check if an index file has been opened, and if not, open it. \def\requireopenindexfile#1{% \ifnum\csname #1indfile\endcsname=0 \expandafter\newwrite \csname#1indfile\endcsname \edef\suffix{#1}% % A .fls suffix would conflict with the file extension for the output % of -recorder, so use .f1s instead. \ifx\suffix\indexisfl\def\suffix{f1}\fi % Open the file \immediate\openout\csname#1indfile\endcsname \jobname.\suffix % Using \immediate above here prevents an object entering into the current % box, which could confound checks such as those in \safewhatsit for % preceding skips. \typeout{Writing index file \jobname.\suffix}% \fi} \def\indexisfl{fl} % Output \ as {\indexbackslash}, because \ is an escape character in % the index files. \let\indexbackslash=\relax {\catcode`\@=0 \catcode`\\=\active @gdef@useindexbackslash{@def\{{@indexbackslash}}} } % Definition for writing index entry text. \def\sortas#1{\ignorespaces}% % Definition for writing index entry sort key. Should occur at the at % the beginning of the index entry, like % @cindex @sortas{september} \september % The \ignorespaces takes care of following space, but there's no way % to remove space before it. { \catcode`\-=13 \gdef\indexwritesortas{% \begingroup \indexnonalnumreappear \indexwritesortasxxx} \gdef\indexwritesortasxxx#1{% \xdef\indexsortkey{#1}\endgroup} } % Write the entry in \toks0 to the index file. % \def\dosubindwrite{% % Put the index entry in the margin if desired. \ifx\SETmarginindex\relax\else \insert\margin{\hbox{\vrule height8pt depth3pt width0pt \the\toks0}}% \fi % % Remember, we are within a group. \indexdummies % Must do this here, since \bf, etc expand at this stage \useindexbackslash % \indexbackslash isn't defined now so it will be output % as is; and it will print as backslash. % The braces around \indexbrace are recognized by texindex. % % Get the string to sort by, by processing the index entry with all % font commands turned off. {\indexnofonts \def\lbracechar{{\indexlbrace}}% \def\rbracechar{{\indexrbrace}}% \let\{=\lbracechar \let\}=\rbracechar \indexnonalnumdisappear \xdef\indexsortkey{}% \let\sortas=\indexwritesortas \edef\temp{\the\toks0}% \setbox\dummybox = \hbox{\temp}% Make sure to execute any \sortas \ifx\indexsortkey\empty \xdef\indexsortkey{\temp}% \ifx\indexsortkey\empty\xdef\indexsortkey{ }\fi \fi }% % % Set up the complete index entry, with both the sort key and % the original text, including any font commands. We write % three arguments to \entry to the .?? file (four in the % subentry case), texindex reduces to two when writing the .??s % sorted result. \edef\temp{% \write\writeto{% \string\entry{\indexsortkey}{\noexpand\folio}{\the\toks0}}% }% \temp } \newbox\dummybox % used above % Take care of unwanted page breaks/skips around a whatsit: % % If a skip is the last thing on the list now, preserve it % by backing up by \lastskip, doing the \write, then inserting % the skip again. Otherwise, the whatsit generated by the % \write or \pdfdest will make \lastskip zero. The result is that % sequences like this: % @end defun % @tindex whatever % @defun ... % will have extra space inserted, because the \medbreak in the % start of the @defun won't see the skip inserted by the @end of % the previous defun. % % But don't do any of this if we're not in vertical mode. We % don't want to do a \vskip and prematurely end a paragraph. % % Avoid page breaks due to these extra skips, too. % % But wait, there is a catch there: % We'll have to check whether \lastskip is zero skip. \ifdim is not % sufficient for this purpose, as it ignores stretch and shrink parts % of the skip. The only way seems to be to check the textual % representation of the skip. % % The following is almost like \def\zeroskipmacro{0.0pt} except that % the ``p'' and ``t'' characters have catcode \other, not 11 (letter). % \edef\zeroskipmacro{\expandafter\the\csname z@skip\endcsname} % \newskip\whatsitskip \newcount\whatsitpenalty % % ..., ready, GO: % \def\safewhatsit#1{\ifhmode #1% \else % \lastskip and \lastpenalty cannot both be nonzero simultaneously. \whatsitskip = \lastskip \edef\lastskipmacro{\the\lastskip}% \whatsitpenalty = \lastpenalty % % If \lastskip is nonzero, that means the last item was a % skip. And since a skip is discardable, that means this % -\whatsitskip glue we're inserting is preceded by a % non-discardable item, therefore it is not a potential % breakpoint, therefore no \nobreak needed. \ifx\lastskipmacro\zeroskipmacro \else \vskip-\whatsitskip \fi % #1% % \ifx\lastskipmacro\zeroskipmacro % If \lastskip was zero, perhaps the last item was a penalty, and % perhaps it was >=10000, e.g., a \nobreak. In that case, we want % to re-insert the same penalty (values >10000 are used for various % signals); since we just inserted a non-discardable item, any % following glue (such as a \parskip) would be a breakpoint. For example: % @deffn deffn-whatever % @vindex index-whatever % Description. % would allow a break between the index-whatever whatsit % and the "Description." paragraph. \ifnum\whatsitpenalty>9999 \penalty\whatsitpenalty \fi \else % On the other hand, if we had a nonzero \lastskip, % this make-up glue would be preceded by a non-discardable item % (the whatsit from the \write), so we must insert a \nobreak. \nobreak\vskip\whatsitskip \fi \fi} % The index entry written in the file actually looks like % \entry {sortstring}{page}{topic} % or % \entry {sortstring}{page}{topic}{subtopic} % The texindex program reads in these files and writes files % containing these kinds of lines: % \initial {c} % before the first topic whose initial is c % \entry {topic}{pagelist} % for a topic that is used without subtopics % \primary {topic} % for the beginning of a topic that is used with subtopics % \secondary {subtopic}{pagelist} % for each subtopic. % Define the user-accessible indexing commands % @findex, @vindex, @kindex, @cindex. \def\findex {\fnindex} \def\kindex {\kyindex} \def\cindex {\cpindex} \def\vindex {\vrindex} \def\tindex {\tpindex} \def\pindex {\pgindex} \def\cindexsub {\begingroup\obeylines\cindexsub} {\obeylines % \gdef\cindexsub "#1" #2^^M{\endgroup % \dosubind{cp}{#2}{#1}}} % Define the macros used in formatting output of the sorted index material. % @printindex causes a particular index (the ??s file) to get printed. % It does not print any chapter heading (usually an @unnumbered). % \parseargdef\printindex{\begingroup \dobreak \chapheadingskip{10000}% % \smallfonts \rm \tolerance = 9500 \plainfrenchspacing \everypar = {}% don't want the \kern\-parindent from indentation suppression. % % See if the index file exists and is nonempty. % Change catcode of @ here so that if the index file contains % \initial {@} % as its first line, TeX doesn't complain about mismatched braces % (because it thinks @} is a control sequence). \catcode`\@ = 12 % See comment in \requireopenindexfile. \def\indexname{#1}\ifx\indexname\indexisfl\def\indexname{f1}\fi \openin 1 \jobname.\indexname s \ifeof 1 % \enddoublecolumns gets confused if there is no text in the index, % and it loses the chapter title and the aux file entries for the % index. The easiest way to prevent this problem is to make sure % there is some text. \putwordIndexNonexistent \typeout{No file \jobname.\indexname s.}% \else \catcode`\\ = 0 % % If the index file exists but is empty, then \openin leaves \ifeof % false. We have to make TeX try to read something from the file, so % it can discover if there is anything in it. \read 1 to \thisline \ifeof 1 \putwordIndexIsEmpty \else % Index files are almost Texinfo source, but we use \ as the escape % character. It would be better to use @, but that's too big a change % to make right now. \def\indexbackslash{\ttbackslash}% \let\indexlbrace\{ % Likewise, set these sequences for braces \let\indexrbrace\} % used in the sort key. \begindoublecolumns \let\entrywidowpenalty=\indexwidowpenalty % % Read input from the index file line by line. \loopdo \ifeof1 \let\firsttoken\relax \else \read 1 to \nextline \edef\act{\gdef\noexpand\firsttoken{\getfirsttoken\nextline}}% \act \fi \thisline % \ifeof1\else \let\thisline\nextline \repeat %% \enddoublecolumns \fi \fi \closein 1 \endgroup} \def\getfirsttoken#1{\expandafter\getfirsttokenx#1\endfirsttoken} \long\def\getfirsttokenx#1#2\endfirsttoken{\noexpand#1} \def\loopdo#1\repeat{\def\body{#1}\loopdoxxx} \def\loopdoxxx{\let\next=\relax\body\let\next=\loopdoxxx\fi\next} % These macros are used by the sorted index file itself. % Change them to control the appearance of the index. {\catcode`\/=13 \catcode`\-=13 \catcode`\^=13 \catcode`\~=13 \catcode`\_=13 \catcode`\|=13 \catcode`\<=13 \catcode`\>=13 \catcode`\+=13 \catcode`\"=13 \catcode`\$=3 \gdef\initialglyphs{% % Some changes for non-alphabetic characters. Using the glyphs from the % math fonts looks more consistent than the typewriter font used elsewhere % for these characters. \def\indexbackslash{\math{\backslash}}% \let\\=\indexbackslash % % Can't get bold backslash so don't use bold forward slash \catcode`\/=13 \def/{{\secrmnotbold \normalslash}}% \def-{{\normaldash\normaldash}}% en dash `--' \def^{{\chapbf \normalcaret}}% \def~{{\chapbf \normaltilde}}% \def\_{% \leavevmode \kern.07em \vbox{\hrule width.3em height.1ex}\kern .07em }% \def|{$\vert$}% \def<{$\less$}% \def>{$\gtr$}% \def+{$\normalplus$}% }} \def\initial{% \bgroup \initialglyphs \initialx } \def\initialx#1{% % Remove any glue we may have, we'll be inserting our own. \removelastskip % % We like breaks before the index initials, so insert a bonus. % The glue before the bonus allows a little bit of space at the % bottom of a column to reduce an increase in inter-line spacing. \nobreak \vskip 0pt plus 5\baselineskip \penalty -300 \vskip 0pt plus -5\baselineskip % % Typeset the initial. Making this add up to a whole number of % baselineskips increases the chance of the dots lining up from column % to column. It still won't often be perfect, because of the stretch % we need before each entry, but it's better. % % No shrink because it confuses \balancecolumns. \vskip 1.67\baselineskip plus 1\baselineskip \leftline{\secfonts \kern-0.05em \secbf #1}% % \secfonts is inside the argument of \leftline so that the change of % \baselineskip will not affect any glue inserted before the vbox that % \leftline creates. % Do our best not to break after the initial. \nobreak \vskip .33\baselineskip plus .1\baselineskip \egroup % \initialglyphs } \newdimen\entryrightmargin \entryrightmargin=0pt % \entry typesets a paragraph consisting of the text (#1), dot leaders, and % then page number (#2) flushed to the right margin. It is used for index % and table of contents entries. The paragraph is indented by \leftskip. % \def\entry{% \begingroup % % For pdfTeX and XeTeX. % The redefinition of \domark stops marks being added in \pdflink to % preserve coloured links across page boundaries. Otherwise the marks % would get in the way of \lastbox in \insertindexentrybox. \let\domark\relax % % Start a new paragraph if necessary, so our assignments below can't % affect previous text. \par % % No extra space above this paragraph. \parskip = 0in % % When reading the text of entry, convert explicit line breaks % from @* into spaces. The user might give these in long section % titles, for instance. \def\*{\unskip\space\ignorespaces}% \def\entrybreak{\hfil\break}% An undocumented command % % Swallow the left brace of the text (first parameter): \afterassignment\doentry \let\temp = } \def\entrybreak{\unskip\space\ignorespaces}% \def\doentry{% % Save the text of the entry \global\setbox\boxA=\hbox\bgroup \bgroup % Instead of the swallowed brace. \noindent \aftergroup\finishentry % And now comes the text of the entry. % Not absorbing as a macro argument reduces the chance of problems % with catcodes occurring. } {\catcode`\@=11 \gdef\finishentry#1{% \egroup % end box A \dimen@ = \wd\boxA % Length of text of entry \global\setbox\boxA=\hbox\bgroup\unhbox\boxA % #1 is the page number. % % Get the width of the page numbers, and only use % leaders if they are present. \global\setbox\boxB = \hbox{#1}% \ifdim\wd\boxB = 0pt \null\nobreak\hfill\ % \else % \null\nobreak\indexdotfill % Have leaders before the page number. % \ifpdf \pdfgettoks#1.% \hskip\skip\thinshrinkable\the\toksA \else \ifx\XeTeXrevision\thisisundefined \hskip\skip\thinshrinkable #1% \else \pdfgettoks#1.% \hskip\skip\thinshrinkable\the\toksA \fi \fi \fi \egroup % end \boxA \ifdim\wd\boxB = 0pt \global\setbox\entryindexbox=\vbox{\unhbox\boxA}% \else \global\setbox\entryindexbox=\vbox\bgroup % We want the text of the entries to be aligned to the left, and the % page numbers to be aligned to the right. % \parindent = 0pt \advance\leftskip by 0pt plus 1fil \advance\leftskip by 0pt plus -1fill \rightskip = 0pt plus -1fil \advance\rightskip by 0pt plus 1fill % Cause last line, which could consist of page numbers on their own % if the list of page numbers is long, to be aligned to the right. \parfillskip=0pt plus -1fill % \advance\rightskip by \entryrightmargin % Determine how far we can stretch into the margin. % This allows, e.g., "Appendix H GNU Free Documentation License" to % fit on one line in @letterpaper format. \ifdim\entryrightmargin>2.1em \dimen@i=2.1em \else \dimen@i=0em \fi \advance \parfillskip by 0pt minus 1\dimen@i % \dimen@ii = \hsize \advance\dimen@ii by -1\leftskip \advance\dimen@ii by -1\entryrightmargin \advance\dimen@ii by 1\dimen@i \ifdim\wd\boxA > \dimen@ii % If the entry doesn't fit in one line \ifdim\dimen@ > 0.8\dimen@ii % due to long index text \dimen@ = 0.7\dimen@ % Try to split the text roughly evenly \dimen@ii = \hsize \ifnum\dimen@>\dimen@ii % If the entry is too long, use the whole line \dimen@ = \dimen@ii \fi \advance\leftskip by 0pt plus 1fill % ragged right \advance \dimen@ by 1\rightskip \parshape = 2 0pt \dimen@ 0em \dimen@ii % Ideally we'd add a finite glue at the end of the first line only, % instead of using \parshape with explicit line lengths, but TeX % doesn't seem to provide a way to do such a thing. % \leftskip = 1em \parindent = -1em \fi\fi \indent % start paragraph \unhbox\boxA % % Do not prefer a separate line ending with a hyphen to fewer lines. \finalhyphendemerits = 0 % % Word spacing - no stretch \spaceskip=\fontdimen2\font minus \fontdimen4\font % \linepenalty=1000 % Discourage line breaks. \hyphenpenalty=5000 % Discourage hyphenation. % \par % format the paragraph \egroup % The \vbox \fi \endgroup % delay text of entry until after penalty \bgroup\aftergroup\insertindexentrybox \entrywidowpenalty }} \newskip\thinshrinkable \skip\thinshrinkable=.15em minus .15em \newbox\entryindexbox \def\insertindexentrybox{% \ourunvbox\entryindexbox } % Use \lastbox to take apart vbox box by box, and add each sub-box % to the current vertical list. \def\ourunvbox#1{% \bgroup % for local binding of \delayedbox % Remove the last box from box #1 \global\setbox#1=\vbox{% \unvbox#1% \unskip % remove any glue \unpenalty \global\setbox\interbox=\lastbox }% \setbox\delayedbox=\box\interbox \ifdim\ht#1=0pt\else \ourunvbox#1 % Repeat on what's left of the box \nobreak \fi \box\delayedbox \egroup } \newbox\delayedbox \newbox\interbox % Default is no penalty \let\entrywidowpenalty\egroup % Used from \printindex. \firsttoken should be the first token % after the \entry. If it's not another \entry, we are at the last % line of a group of index entries, so insert a penalty to discourage % widowed index entries. \long\def\indexwidowpenalty{% \def\isentry{\entry}% \ifx\firsttoken\isentry \else \penalty 9000 \fi \egroup % now comes the box added with \aftergroup } % Like plain.tex's \dotfill, except uses up at least 1 em. % The filll stretch here overpowers both the fil and fill stretch to push % the page number to the right. \def\indexdotfill{\cleaders \hbox{$\mathsurround=0pt \mkern1.5mu.\mkern1.5mu$}\hskip 1em plus 1filll} \def\primary #1{\line{#1\hfil}} \newskip\secondaryindent \secondaryindent=0.5cm \def\secondary#1#2{{% \parfillskip=0in \parskip=0in \hangindent=1in \hangafter=1 \noindent\hskip\secondaryindent\hbox{#1}\indexdotfill \ifpdf \pdfgettoks#2.\ \the\toksA % The page number ends the paragraph. \else \ifx\XeTeXrevision\thisisundefined #2 \else \pdfgettoks#2.\ \the\toksA % The page number ends the paragraph. \fi \fi \par }} % Define two-column mode, which we use to typeset indexes. % Adapted from the TeXbook, page 416, which is to say, % the manmac.tex format used to print the TeXbook itself. \catcode`\@=11 % private names \newbox\partialpage \newdimen\doublecolumnhsize % Use inside an output routine to save \topmark and \firstmark \def\savemarks{% \global\savedtopmark=\expandafter{\topmark }% \global\savedfirstmark=\expandafter{\firstmark }% } \newtoks\savedtopmark \newtoks\savedfirstmark % Set \topmark and \firstmark for next time \output runs. % Can't be run from withinside \output (because any material % added while an output routine is active, including % penalties, is saved for after it finishes). The page so far % should be empty, otherwise what's on it will be thrown away. \def\restoremarks{% \mark{\the\savedtopmark}% \bgroup\output = {% \setbox\dummybox=\box\PAGE }abc\eject\egroup % "abc" because output routine doesn't fire for a completely empty page. \mark{\the\savedfirstmark}% } \def\begindoublecolumns{\begingroup % ended by \enddoublecolumns % If not much space left on page, start a new page. \ifdim\pagetotal>0.8\vsize\vfill\eject\fi % % Grab any single-column material above us. \output = {% % % Here is a possibility not foreseen in manmac: if we accumulate a % whole lot of material, we might end up calling this \output % routine twice in a row (see the doublecol-lose test, which is % essentially a couple of indexes with @setchapternewpage off). In % that case we just ship out what is in \partialpage with the normal % output routine. Generally, \partialpage will be empty when this % runs and this will be a no-op. See the indexspread.tex test case. \ifvoid\partialpage \else \onepageout{\pagecontents\partialpage}% \fi % \global\setbox\partialpage = \vbox{% % Unvbox the main output page. \unvbox\PAGE \kern-\topskip \kern\baselineskip }% \savemarks }% \eject % run that output routine to set \partialpage \restoremarks % % We recover the two marks that the last output routine saved in order % to propagate the information in marks added around a chapter heading, % which could be otherwise be lost by the time the final page is output. % % % Use the double-column output routine for subsequent pages. \output = {\doublecolumnout}% % % Change the page size parameters. We could do this once outside this % routine, in each of @smallbook, @afourpaper, and the default 8.5x11 % format, but then we repeat the same computation. Repeating a couple % of assignments once per index is clearly meaningless for the % execution time, so we may as well do it in one place. % % First we halve the line length, less a little for the gutter between % the columns. We compute the gutter based on the line length, so it % changes automatically with the paper format. The magic constant % below is chosen so that the gutter has the same value (well, +-<1pt) % as it did when we hard-coded it. % % We put the result in a separate register, \doublecolumhsize, so we % can restore it in \pagesofar, after \hsize itself has (potentially) % been clobbered. % \doublecolumnhsize = \hsize \advance\doublecolumnhsize by -.04154\hsize \divide\doublecolumnhsize by 2 \hsize = \doublecolumnhsize % % Double the \vsize as well. (We don't need a separate register here, % since nobody clobbers \vsize.) \vsize = 2\vsize % % For the benefit of balancing columns \advance\baselineskip by 0pt plus 0.5pt } % The double-column output routine for all double-column pages except % the last, which is done by \balancecolumns. % \def\doublecolumnout{% % \splittopskip=\topskip \splitmaxdepth=\maxdepth % Get the available space for the double columns -- the normal % (undoubled) page height minus any material left over from the % previous page. \dimen@ = \vsize \divide\dimen@ by 2 \advance\dimen@ by -\ht\partialpage % % box0 will be the left-hand column, box2 the right. \setbox0=\vsplit255 to\dimen@ \setbox2=\vsplit255 to\dimen@ \onepageout\pagesofar \unvbox255 \penalty\outputpenalty } % % Re-output the contents of the output page -- any previous material, % followed by the two boxes we just split, in box0 and box2. \def\pagesofar{% \unvbox\partialpage % \hsize = \doublecolumnhsize \wd0=\hsize \wd2=\hsize \hbox to\txipagewidth{\box0\hfil\box2}% } % Finished with with double columns. \def\enddoublecolumns{% % The following penalty ensures that the page builder is exercised % _before_ we change the output routine. This is necessary in the % following situation: % % The last section of the index consists only of a single entry. % Before this section, \pagetotal is less than \pagegoal, so no % break occurs before the last section starts. However, the last % section, consisting of \initial and the single \entry, does not % fit on the page and has to be broken off. Without the following % penalty the page builder will not be exercised until \eject % below, and by that time we'll already have changed the output % routine to the \balancecolumns version, so the next-to-last % double-column page will be processed with \balancecolumns, which % is wrong: The two columns will go to the main vertical list, with % the broken-off section in the recent contributions. As soon as % the output routine finishes, TeX starts reconsidering the page % break. The two columns and the broken-off section both fit on the % page, because the two columns now take up only half of the page % goal. When TeX sees \eject from below which follows the final % section, it invokes the new output routine that we've set after % \balancecolumns below; \onepageout will try to fit the two columns % and the final section into the vbox of \txipageheight (see % \pagebody), causing an overfull box. % % Note that glue won't work here, because glue does not exercise the % page builder, unlike penalties (see The TeXbook, pp. 280-281). \penalty0 % \output = {% % Split the last of the double-column material. \savemarks \balancecolumns % % Having called \balancecolumns once, we do not % want to call it again. Therefore, reset \output to its normal % definition right away. \global\output = {\onepageout{\pagecontents\PAGE}}% }% \eject \endgroup % started in \begindoublecolumns \restoremarks % Leave the double-column material on the current page, no automatic % page break. \box\balancedcolumns % % \pagegoal was set to the doubled \vsize above, since we restarted % the current page. We're now back to normal single-column % typesetting, so reset \pagegoal to the normal \vsize (after the % \endgroup where \vsize got restored). \pagegoal = \vsize } \newbox\balancedcolumns \setbox\balancedcolumns=\vbox{shouldnt see this}% % % Only called for the last of the double column material. \doublecolumnout % does the others. \def\balancecolumns{% \setbox0 = \vbox{\unvbox255}% like \box255 but more efficient, see p.120. \dimen@ = \ht0 \advance\dimen@ by \topskip \advance\dimen@ by-\baselineskip \ifdim\dimen@<5\baselineskip % Don't split a short final column in two. \setbox2=\vbox{}% \else \divide\dimen@ by 2 % target to split to \dimen@ii = \dimen@ \splittopskip = \topskip % Loop until left column is at least as high as the right column. {% \vbadness = 10000 \loop \global\setbox3 = \copy0 \global\setbox1 = \vsplit3 to \dimen@ \ifdim\ht1<\ht3 \global\advance\dimen@ by 1pt \repeat }% % Now the left column is in box 1, and the right column in box 3. % Check whether the left column has come out higher than the page itself. % (Note that we have doubled \vsize for the double columns, so % the actual height of the page is 0.5\vsize). \ifdim2\ht1>\vsize % Just split the last of the double column material roughly in half. \setbox2=\box0 \setbox0 = \vsplit2 to \dimen@ii \setbox0=\vbox to \dimen@ii {\unvbox0\vfill}% \setbox2=\vbox to \dimen@ii {\unvbox2\vfill}% \else % Compare the heights of the two columns. \ifdim4\ht1>5\ht3 % Column heights are too different, so don't make their bottoms % flush with each other. \setbox2=\vbox to \ht1 {\unvbox3\vfill}% \setbox0=\vbox to \ht1 {\unvbox1\vfill}% \else % Make column bottoms flush with each other. \setbox2=\vbox to\ht1{\unvbox3\unskip}% \setbox0=\vbox to\ht1{\unvbox1\unskip}% \fi \fi \fi % \global\setbox\balancedcolumns=\vbox{\pagesofar}% } \catcode`\@ = \other \message{sectioning,} % Chapters, sections, etc. % Let's start with @part. \outer\parseargdef\part{\partzzz{#1}} \def\partzzz#1{% \chapoddpage \null \vskip.3\vsize % move it down on the page a bit \begingroup \noindent \titlefonts\rm #1\par % the text \let\lastnode=\empty % no node to associate with \writetocentry{part}{#1}{}% but put it in the toc \headingsoff % no headline or footline on the part page % This outputs a mark at the end of the page that clears \thischapter % and \thissection, as is done in \startcontents. \let\pchapsepmacro\relax \chapmacro{}{Yomitfromtoc}{}% \chapoddpage \endgroup } % \unnumberedno is an oxymoron. But we count the unnumbered % sections so that we can refer to them unambiguously in the pdf % outlines by their "section number". We avoid collisions with chapter % numbers by starting them at 10000. (If a document ever has 10000 % chapters, we're in trouble anyway, I'm sure.) \newcount\unnumberedno \unnumberedno = 10000 \newcount\chapno \newcount\secno \secno=0 \newcount\subsecno \subsecno=0 \newcount\subsubsecno \subsubsecno=0 % This counter is funny since it counts through charcodes of letters A, B, ... \newcount\appendixno \appendixno = `\@ % % \def\appendixletter{\char\the\appendixno} % We do the following ugly conditional instead of the above simple % construct for the sake of pdftex, which needs the actual % letter in the expansion, not just typeset. % \def\appendixletter{% \ifnum\appendixno=`A A% \else\ifnum\appendixno=`B B% \else\ifnum\appendixno=`C C% \else\ifnum\appendixno=`D D% \else\ifnum\appendixno=`E E% \else\ifnum\appendixno=`F F% \else\ifnum\appendixno=`G G% \else\ifnum\appendixno=`H H% \else\ifnum\appendixno=`I I% \else\ifnum\appendixno=`J J% \else\ifnum\appendixno=`K K% \else\ifnum\appendixno=`L L% \else\ifnum\appendixno=`M M% \else\ifnum\appendixno=`N N% \else\ifnum\appendixno=`O O% \else\ifnum\appendixno=`P P% \else\ifnum\appendixno=`Q Q% \else\ifnum\appendixno=`R R% \else\ifnum\appendixno=`S S% \else\ifnum\appendixno=`T T% \else\ifnum\appendixno=`U U% \else\ifnum\appendixno=`V V% \else\ifnum\appendixno=`W W% \else\ifnum\appendixno=`X X% \else\ifnum\appendixno=`Y Y% \else\ifnum\appendixno=`Z Z% % The \the is necessary, despite appearances, because \appendixletter is % expanded while writing the .toc file. \char\appendixno is not % expandable, thus it is written literally, thus all appendixes come out % with the same letter (or @) in the toc without it. \else\char\the\appendixno \fi\fi\fi\fi\fi\fi\fi\fi\fi\fi\fi\fi\fi \fi\fi\fi\fi\fi\fi\fi\fi\fi\fi\fi\fi\fi} % Each @chapter defines these (using marks) as the number+name, number % and name of the chapter. Page headings and footings can use % these. @section does likewise. \def\thischapter{} \def\thischapternum{} \def\thischaptername{} \def\thissection{} \def\thissectionnum{} \def\thissectionname{} \newcount\absseclevel % used to calculate proper heading level \newcount\secbase\secbase=0 % @raisesections/@lowersections modify this count % @raisesections: treat @section as chapter, @subsection as section, etc. \def\raisesections{\global\advance\secbase by -1} \let\up=\raisesections % original BFox name % @lowersections: treat @chapter as section, @section as subsection, etc. \def\lowersections{\global\advance\secbase by 1} \let\down=\lowersections % original BFox name % we only have subsub. \chardef\maxseclevel = 3 % % A numbered section within an unnumbered changes to unnumbered too. % To achieve this, remember the "biggest" unnum. sec. we are currently in: \chardef\unnlevel = \maxseclevel % % Trace whether the current chapter is an appendix or not: % \chapheadtype is "N" or "A", unnumbered chapters are ignored. \def\chapheadtype{N} % Choose a heading macro % #1 is heading type % #2 is heading level % #3 is text for heading \def\genhead#1#2#3{% % Compute the abs. sec. level: \absseclevel=#2 \advance\absseclevel by \secbase % Make sure \absseclevel doesn't fall outside the range: \ifnum \absseclevel < 0 \absseclevel = 0 \else \ifnum \absseclevel > 3 \absseclevel = 3 \fi \fi % The heading type: \def\headtype{#1}% \if \headtype U% \ifnum \absseclevel < \unnlevel \chardef\unnlevel = \absseclevel \fi \else % Check for appendix sections: \ifnum \absseclevel = 0 \edef\chapheadtype{\headtype}% \else \if \headtype A\if \chapheadtype N% \errmessage{@appendix... within a non-appendix chapter}% \fi\fi \fi % Check for numbered within unnumbered: \ifnum \absseclevel > \unnlevel \def\headtype{U}% \else \chardef\unnlevel = 3 \fi \fi % Now print the heading: \if \headtype U% \ifcase\absseclevel \unnumberedzzz{#3}% \or \unnumberedseczzz{#3}% \or \unnumberedsubseczzz{#3}% \or \unnumberedsubsubseczzz{#3}% \fi \else \if \headtype A% \ifcase\absseclevel \appendixzzz{#3}% \or \appendixsectionzzz{#3}% \or \appendixsubseczzz{#3}% \or \appendixsubsubseczzz{#3}% \fi \else \ifcase\absseclevel \chapterzzz{#3}% \or \seczzz{#3}% \or \numberedsubseczzz{#3}% \or \numberedsubsubseczzz{#3}% \fi \fi \fi \suppressfirstparagraphindent } % an interface: \def\numhead{\genhead N} \def\apphead{\genhead A} \def\unnmhead{\genhead U} % @chapter, @appendix, @unnumbered. Increment top-level counter, reset % all lower-level sectioning counters to zero. % % Also set \chaplevelprefix, which we prepend to @float sequence numbers % (e.g., figures), q.v. By default (before any chapter), that is empty. \let\chaplevelprefix = \empty % \outer\parseargdef\chapter{\numhead0{#1}} % normally numhead0 calls chapterzzz \def\chapterzzz#1{% % section resetting is \global in case the chapter is in a group, such % as an @include file. \global\secno=0 \global\subsecno=0 \global\subsubsecno=0 \global\advance\chapno by 1 % % Used for \float. \gdef\chaplevelprefix{\the\chapno.}% \resetallfloatnos % % \putwordChapter can contain complex things in translations. \toks0=\expandafter{\putwordChapter}% \message{\the\toks0 \space \the\chapno}% % % Write the actual heading. \chapmacro{#1}{Ynumbered}{\the\chapno}% % % So @section and the like are numbered underneath this chapter. \global\let\section = \numberedsec \global\let\subsection = \numberedsubsec \global\let\subsubsection = \numberedsubsubsec } \outer\parseargdef\appendix{\apphead0{#1}} % normally calls appendixzzz % \def\appendixzzz#1{% \global\secno=0 \global\subsecno=0 \global\subsubsecno=0 \global\advance\appendixno by 1 \gdef\chaplevelprefix{\appendixletter.}% \resetallfloatnos % % \putwordAppendix can contain complex things in translations. \toks0=\expandafter{\putwordAppendix}% \message{\the\toks0 \space \appendixletter}% % \chapmacro{#1}{Yappendix}{\appendixletter}% % \global\let\section = \appendixsec \global\let\subsection = \appendixsubsec \global\let\subsubsection = \appendixsubsubsec } % normally unnmhead0 calls unnumberedzzz: \outer\parseargdef\unnumbered{\unnmhead0{#1}} \def\unnumberedzzz#1{% \global\secno=0 \global\subsecno=0 \global\subsubsecno=0 \global\advance\unnumberedno by 1 % % Since an unnumbered has no number, no prefix for figures. \global\let\chaplevelprefix = \empty \resetallfloatnos % % This used to be simply \message{#1}, but TeX fully expands the % argument to \message. Therefore, if #1 contained @-commands, TeX % expanded them. For example, in `@unnumbered The @cite{Book}', TeX % expanded @cite (which turns out to cause errors because \cite is meant % to be executed, not expanded). % % Anyway, we don't want the fully-expanded definition of @cite to appear % as a result of the \message, we just want `@cite' itself. We use % \the<toks register> to achieve this: TeX expands \the<toks> only once, % simply yielding the contents of <toks register>. (We also do this for % the toc entries.) \toks0 = {#1}% \message{(\the\toks0)}% % \chapmacro{#1}{Ynothing}{\the\unnumberedno}% % \global\let\section = \unnumberedsec \global\let\subsection = \unnumberedsubsec \global\let\subsubsection = \unnumberedsubsubsec } % @centerchap is like @unnumbered, but the heading is centered. \outer\parseargdef\centerchap{% \let\centerparametersmaybe = \centerparameters \unnmhead0{#1}% \let\centerparametersmaybe = \relax } % @top is like @unnumbered. \let\top\unnumbered % Sections. % \outer\parseargdef\numberedsec{\numhead1{#1}} % normally calls seczzz \def\seczzz#1{% \global\subsecno=0 \global\subsubsecno=0 \global\advance\secno by 1 \sectionheading{#1}{sec}{Ynumbered}{\the\chapno.\the\secno}% } % normally calls appendixsectionzzz: \outer\parseargdef\appendixsection{\apphead1{#1}} \def\appendixsectionzzz#1{% \global\subsecno=0 \global\subsubsecno=0 \global\advance\secno by 1 \sectionheading{#1}{sec}{Yappendix}{\appendixletter.\the\secno}% } \let\appendixsec\appendixsection % normally calls unnumberedseczzz: \outer\parseargdef\unnumberedsec{\unnmhead1{#1}} \def\unnumberedseczzz#1{% \global\subsecno=0 \global\subsubsecno=0 \global\advance\secno by 1 \sectionheading{#1}{sec}{Ynothing}{\the\unnumberedno.\the\secno}% } % Subsections. % % normally calls numberedsubseczzz: \outer\parseargdef\numberedsubsec{\numhead2{#1}} \def\numberedsubseczzz#1{% \global\subsubsecno=0 \global\advance\subsecno by 1 \sectionheading{#1}{subsec}{Ynumbered}{\the\chapno.\the\secno.\the\subsecno}% } % normally calls appendixsubseczzz: \outer\parseargdef\appendixsubsec{\apphead2{#1}} \def\appendixsubseczzz#1{% \global\subsubsecno=0 \global\advance\subsecno by 1 \sectionheading{#1}{subsec}{Yappendix}% {\appendixletter.\the\secno.\the\subsecno}% } % normally calls unnumberedsubseczzz: \outer\parseargdef\unnumberedsubsec{\unnmhead2{#1}} \def\unnumberedsubseczzz#1{% \global\subsubsecno=0 \global\advance\subsecno by 1 \sectionheading{#1}{subsec}{Ynothing}% {\the\unnumberedno.\the\secno.\the\subsecno}% } % Subsubsections. % % normally numberedsubsubseczzz: \outer\parseargdef\numberedsubsubsec{\numhead3{#1}} \def\numberedsubsubseczzz#1{% \global\advance\subsubsecno by 1 \sectionheading{#1}{subsubsec}{Ynumbered}% {\the\chapno.\the\secno.\the\subsecno.\the\subsubsecno}% } % normally appendixsubsubseczzz: \outer\parseargdef\appendixsubsubsec{\apphead3{#1}} \def\appendixsubsubseczzz#1{% \global\advance\subsubsecno by 1 \sectionheading{#1}{subsubsec}{Yappendix}% {\appendixletter.\the\secno.\the\subsecno.\the\subsubsecno}% } % normally unnumberedsubsubseczzz: \outer\parseargdef\unnumberedsubsubsec{\unnmhead3{#1}} \def\unnumberedsubsubseczzz#1{% \global\advance\subsubsecno by 1 \sectionheading{#1}{subsubsec}{Ynothing}% {\the\unnumberedno.\the\secno.\the\subsecno.\the\subsubsecno}% } % These macros control what the section commands do, according % to what kind of chapter we are in (ordinary, appendix, or unnumbered). % Define them by default for a numbered chapter. \let\section = \numberedsec \let\subsection = \numberedsubsec \let\subsubsection = \numberedsubsubsec % Define @majorheading, @heading and @subheading \def\majorheading{% {\advance\chapheadingskip by 10pt \chapbreak }% \parsearg\chapheadingzzz } \def\chapheading{\chapbreak \parsearg\chapheadingzzz} \def\chapheadingzzz#1{% \vbox{\chapfonts \raggedtitlesettings #1\par}% \nobreak\bigskip \nobreak \suppressfirstparagraphindent } % @heading, @subheading, @subsubheading. \parseargdef\heading{\sectionheading{#1}{sec}{Yomitfromtoc}{} \suppressfirstparagraphindent} \parseargdef\subheading{\sectionheading{#1}{subsec}{Yomitfromtoc}{} \suppressfirstparagraphindent} \parseargdef\subsubheading{\sectionheading{#1}{subsubsec}{Yomitfromtoc}{} \suppressfirstparagraphindent} % These macros generate a chapter, section, etc. heading only % (including whitespace, linebreaking, etc. around it), % given all the information in convenient, parsed form. % Args are the skip and penalty (usually negative) \def\dobreak#1#2{\par\ifdim\lastskip<#1\removelastskip\penalty#2\vskip#1\fi} % Parameter controlling skip before chapter headings (if needed) \newskip\chapheadingskip % Define plain chapter starts, and page on/off switching for it. \def\chapbreak{\dobreak \chapheadingskip {-4000}} % Start a new page \def\chappager{\par\vfill\supereject} % \chapoddpage - start on an odd page for a new chapter % Because \domark is called before \chapoddpage, the filler page will % get the headings for the next chapter, which is wrong. But we don't % care -- we just disable all headings on the filler page. \def\chapoddpage{% \chappager \ifodd\pageno \else \begingroup \headingsoff \null \chappager \endgroup \fi } \parseargdef\setchapternewpage{\csname CHAPPAG#1\endcsname} \def\CHAPPAGoff{% \global\let\contentsalignmacro = \chappager \global\let\pchapsepmacro=\chapbreak \global\let\pagealignmacro=\chappager} \def\CHAPPAGon{% \global\let\contentsalignmacro = \chappager \global\let\pchapsepmacro=\chappager \global\let\pagealignmacro=\chappager \global\def\HEADINGSon{\HEADINGSsingle}} \def\CHAPPAGodd{% \global\let\contentsalignmacro = \chapoddpage \global\let\pchapsepmacro=\chapoddpage \global\let\pagealignmacro=\chapoddpage \global\def\HEADINGSon{\HEADINGSdouble}} \CHAPPAGon % \chapmacro - Chapter opening. % % #1 is the text, #2 is the section type (Ynumbered, Ynothing, % Yappendix, Yomitfromtoc), #3 the chapter number. % Not used for @heading series. % % To test against our argument. \def\Ynothingkeyword{Ynothing} \def\Yappendixkeyword{Yappendix} \def\Yomitfromtockeyword{Yomitfromtoc} % \def\chapmacro#1#2#3{% \expandafter\ifx\thisenv\titlepage\else \checkenv{}% chapters, etc., should not start inside an environment. \fi % FIXME: \chapmacro is currently called from inside \titlepage when % \setcontentsaftertitlepage to print the "Table of Contents" heading, but % this should probably be done by \sectionheading with an option to print % in chapter size. % % Insert the first mark before the heading break (see notes for \domark). \let\prevchapterdefs=\lastchapterdefs \let\prevsectiondefs=\lastsectiondefs \gdef\lastsectiondefs{\gdef\thissectionname{}\gdef\thissectionnum{}% \gdef\thissection{}}% % \def\temptype{#2}% \ifx\temptype\Ynothingkeyword \gdef\lastchapterdefs{\gdef\thischaptername{#1}\gdef\thischapternum{}% \gdef\thischapter{\thischaptername}}% \else\ifx\temptype\Yomitfromtockeyword \gdef\lastchapterdefs{\gdef\thischaptername{#1}\gdef\thischapternum{}% \gdef\thischapter{}}% \else\ifx\temptype\Yappendixkeyword \toks0={#1}% \xdef\lastchapterdefs{% \gdef\noexpand\thischaptername{\the\toks0}% \gdef\noexpand\thischapternum{\appendixletter}% % \noexpand\putwordAppendix avoids expanding indigestible % commands in some of the translations. \gdef\noexpand\thischapter{\noexpand\putwordAppendix{} \noexpand\thischapternum: \noexpand\thischaptername}% }% \else \toks0={#1}% \xdef\lastchapterdefs{% \gdef\noexpand\thischaptername{\the\toks0}% \gdef\noexpand\thischapternum{\the\chapno}% % \noexpand\putwordChapter avoids expanding indigestible % commands in some of the translations. \gdef\noexpand\thischapter{\noexpand\putwordChapter{} \noexpand\thischapternum: \noexpand\thischaptername}% }% \fi\fi\fi % % Output the mark. Pass it through \safewhatsit, to take care of % the preceding space. \safewhatsit\domark % % Insert the chapter heading break. \pchapsepmacro % % Now the second mark, after the heading break. No break points % between here and the heading. \let\prevchapterdefs=\lastchapterdefs \let\prevsectiondefs=\lastsectiondefs \domark % {% \chapfonts \rm \let\footnote=\errfootnoteheading % give better error message % % Have to define \lastsection before calling \donoderef, because the % xref code eventually uses it. On the other hand, it has to be called % after \pchapsepmacro, or the headline will change too soon. \gdef\lastsection{#1}% % % Only insert the separating space if we have a chapter/appendix % number, and don't print the unnumbered ``number''. \ifx\temptype\Ynothingkeyword \setbox0 = \hbox{}% \def\toctype{unnchap}% \else\ifx\temptype\Yomitfromtockeyword \setbox0 = \hbox{}% contents like unnumbered, but no toc entry \def\toctype{omit}% \else\ifx\temptype\Yappendixkeyword \setbox0 = \hbox{\putwordAppendix{} #3\enspace}% \def\toctype{app}% \else \setbox0 = \hbox{#3\enspace}% \def\toctype{numchap}% \fi\fi\fi % % Write the toc entry for this chapter. Must come before the % \donoderef, because we include the current node name in the toc % entry, and \donoderef resets it to empty. \writetocentry{\toctype}{#1}{#3}% % % For pdftex, we have to write out the node definition (aka, make % the pdfdest) after any page break, but before the actual text has % been typeset. If the destination for the pdf outline is after the % text, then jumping from the outline may wind up with the text not % being visible, for instance under high magnification. \donoderef{#2}% % % Typeset the actual heading. \nobreak % Avoid page breaks at the interline glue. \vbox{\raggedtitlesettings \hangindent=\wd0 \centerparametersmaybe \unhbox0 #1\par}% }% \nobreak\bigskip % no page break after a chapter title \nobreak } % @centerchap -- centered and unnumbered. \let\centerparametersmaybe = \relax \def\centerparameters{% \advance\rightskip by 3\rightskip \leftskip = \rightskip \parfillskip = 0pt } % Section titles. These macros combine the section number parts and % call the generic \sectionheading to do the printing. % \newskip\secheadingskip \def\secheadingbreak{\dobreak \secheadingskip{-1000}} % Subsection titles. \newskip\subsecheadingskip \def\subsecheadingbreak{\dobreak \subsecheadingskip{-500}} % Subsubsection titles. \def\subsubsecheadingskip{\subsecheadingskip} \def\subsubsecheadingbreak{\subsecheadingbreak} % Print any size, any type, section title. % % #1 is the text of the title, % #2 is the section level (sec/subsec/subsubsec), % #3 is the section type (Ynumbered, Ynothing, Yappendix, Yomitfromtoc), % #4 is the section number. % \def\seckeyword{sec} % \def\sectionheading#1#2#3#4{% {% \def\sectionlevel{#2}% \def\temptype{#3}% % % It is ok for the @heading series commands to appear inside an % environment (it's been historically allowed, though the logic is % dubious), but not the others. \ifx\temptype\Yomitfromtockeyword\else \checkenv{}% non-@*heading should not be in an environment. \fi \let\footnote=\errfootnoteheading % % Switch to the right set of fonts. \csname #2fonts\endcsname \rm % % Insert first mark before the heading break (see notes for \domark). \let\prevsectiondefs=\lastsectiondefs \ifx\temptype\Ynothingkeyword \ifx\sectionlevel\seckeyword \gdef\lastsectiondefs{\gdef\thissectionname{#1}\gdef\thissectionnum{}% \gdef\thissection{\thissectionname}}% \fi \else\ifx\temptype\Yomitfromtockeyword % Don't redefine \thissection. \else\ifx\temptype\Yappendixkeyword \ifx\sectionlevel\seckeyword \toks0={#1}% \xdef\lastsectiondefs{% \gdef\noexpand\thissectionname{\the\toks0}% \gdef\noexpand\thissectionnum{#4}% % \noexpand\putwordSection avoids expanding indigestible % commands in some of the translations. \gdef\noexpand\thissection{\noexpand\putwordSection{} \noexpand\thissectionnum: \noexpand\thissectionname}% }% \fi \else \ifx\sectionlevel\seckeyword \toks0={#1}% \xdef\lastsectiondefs{% \gdef\noexpand\thissectionname{\the\toks0}% \gdef\noexpand\thissectionnum{#4}% % \noexpand\putwordSection avoids expanding indigestible % commands in some of the translations. \gdef\noexpand\thissection{\noexpand\putwordSection{} \noexpand\thissectionnum: \noexpand\thissectionname}% }% \fi \fi\fi\fi % % Go into vertical mode. Usually we'll already be there, but we % don't want the following whatsit to end up in a preceding paragraph % if the document didn't happen to have a blank line. \par % % Output the mark. Pass it through \safewhatsit, to take care of % the preceding space. \safewhatsit\domark % % Insert space above the heading. \csname #2headingbreak\endcsname % % Now the second mark, after the heading break. No break points % between here and the heading. \global\let\prevsectiondefs=\lastsectiondefs \domark % % Only insert the space after the number if we have a section number. \ifx\temptype\Ynothingkeyword \setbox0 = \hbox{}% \def\toctype{unn}% \gdef\lastsection{#1}% \else\ifx\temptype\Yomitfromtockeyword % for @headings -- no section number, don't include in toc, % and don't redefine \lastsection. \setbox0 = \hbox{}% \def\toctype{omit}% \let\sectionlevel=\empty \else\ifx\temptype\Yappendixkeyword \setbox0 = \hbox{#4\enspace}% \def\toctype{app}% \gdef\lastsection{#1}% \else \setbox0 = \hbox{#4\enspace}% \def\toctype{num}% \gdef\lastsection{#1}% \fi\fi\fi % % Write the toc entry (before \donoderef). See comments in \chapmacro. \writetocentry{\toctype\sectionlevel}{#1}{#4}% % % Write the node reference (= pdf destination for pdftex). % Again, see comments in \chapmacro. \donoderef{#3}% % % Interline glue will be inserted when the vbox is completed. % That glue will be a valid breakpoint for the page, since it'll be % preceded by a whatsit (usually from the \donoderef, or from the % \writetocentry if there was no node). We don't want to allow that % break, since then the whatsits could end up on page n while the % section is on page n+1, thus toc/etc. are wrong. Debian bug 276000. \nobreak % % Output the actual section heading. \vbox{\hyphenpenalty=10000 \tolerance=5000 \parindent=0pt \ptexraggedright \hangindent=\wd0 % zero if no section number \unhbox0 #1}% }% % Add extra space after the heading -- half of whatever came above it. % Don't allow stretch, though. \kern .5 \csname #2headingskip\endcsname % % Do not let the kern be a potential breakpoint, as it would be if it % was followed by glue. \nobreak % % We'll almost certainly start a paragraph next, so don't let that % glue accumulate. (Not a breakpoint because it's preceded by a % discardable item.) However, when a paragraph is not started next % (\startdefun, \cartouche, \center, etc.), this needs to be wiped out % or the negative glue will cause weirdly wrong output, typically % obscuring the section heading with something else. \vskip-\parskip % % This is so the last item on the main vertical list is a known % \penalty > 10000, so \startdefun, etc., can recognize the situation % and do the needful. \penalty 10001 } \message{toc,} % Table of contents. \newwrite\tocfile % Write an entry to the toc file, opening it if necessary. % Called from @chapter, etc. % % Example usage: \writetocentry{sec}{Section Name}{\the\chapno.\the\secno} % We append the current node name (if any) and page number as additional % arguments for the \{chap,sec,...}entry macros which will eventually % read this. The node name is used in the pdf outlines as the % destination to jump to. % % We open the .toc file for writing here instead of at @setfilename (or % any other fixed time) so that @contents can be anywhere in the document. % But if #1 is `omit', then we don't do anything. This is used for the % table of contents chapter openings themselves. % \newif\iftocfileopened \def\omitkeyword{omit}% % \def\writetocentry#1#2#3{% \edef\writetoctype{#1}% \ifx\writetoctype\omitkeyword \else \iftocfileopened\else \immediate\openout\tocfile = \jobname.toc \global\tocfileopenedtrue \fi % \iflinks {\atdummies \edef\temp{% \write\tocfile{@#1entry{#2}{#3}{\lastnode}{\noexpand\folio}}}% \temp }% \fi \fi % % Tell \shipout to create a pdf destination on each page, if we're % writing pdf. These are used in the table of contents. We can't % just write one on every page because the title pages are numbered % 1 and 2 (the page numbers aren't printed), and so are the first % two pages of the document. Thus, we'd have two destinations named % `1', and two named `2'. \ifpdf \global\pdfmakepagedesttrue \else \ifx\XeTeXrevision\thisisundefined \else \global\pdfmakepagedesttrue \fi \fi } % These characters do not print properly in the Computer Modern roman % fonts, so we must take special care. This is more or less redundant % with the Texinfo input format setup at the end of this file. % \def\activecatcodes{% \catcode`\"=\active \catcode`\$=\active \catcode`\<=\active \catcode`\>=\active \catcode`\\=\active \catcode`\^=\active \catcode`\_=\active \catcode`\|=\active \catcode`\~=\active } % Read the toc file, which is essentially Texinfo input. \def\readtocfile{% \setupdatafile \activecatcodes \input \tocreadfilename } \newskip\contentsrightmargin \contentsrightmargin=1in \newcount\savepageno \newcount\lastnegativepageno \lastnegativepageno = -1 % Prepare to read what we've written to \tocfile. % \def\startcontents#1{% % If @setchapternewpage on, and @headings double, the contents should % start on an odd page, unlike chapters. Thus, we maintain % \contentsalignmacro in parallel with \pagealignmacro. % From: Torbjorn Granlund <tege@matematik.su.se> \contentsalignmacro \immediate\closeout\tocfile % % Don't need to put `Contents' or `Short Contents' in the headline. % It is abundantly clear what they are. \chapmacro{#1}{Yomitfromtoc}{}% % \savepageno = \pageno \begingroup % Set up to handle contents files properly. \raggedbottom % Worry more about breakpoints than the bottom. \entryrightmargin=\contentsrightmargin % Don't use the full line length. % % Roman numerals for page numbers. \ifnum \pageno>0 \global\pageno = \lastnegativepageno \fi } % redefined for the two-volume lispref. We always output on % \jobname.toc even if this is redefined. % \def\tocreadfilename{\jobname.toc} % Normal (long) toc. % \def\contents{% \startcontents{\putwordTOC}% \openin 1 \tocreadfilename\space \ifeof 1 \else \readtocfile \fi \vfill \eject \contentsalignmacro % in case @setchapternewpage odd is in effect \ifeof 1 \else \pdfmakeoutlines \fi \closein 1 \endgroup \lastnegativepageno = \pageno \global\pageno = \savepageno } % And just the chapters. \def\summarycontents{% \startcontents{\putwordShortTOC}% % \let\partentry = \shortpartentry \let\numchapentry = \shortchapentry \let\appentry = \shortchapentry \let\unnchapentry = \shortunnchapentry % We want a true roman here for the page numbers. \secfonts \let\rm=\shortcontrm \let\bf=\shortcontbf \let\sl=\shortcontsl \let\tt=\shortconttt \rm \hyphenpenalty = 10000 \advance\baselineskip by 1pt % Open it up a little. \def\numsecentry##1##2##3##4{} \let\appsecentry = \numsecentry \let\unnsecentry = \numsecentry \let\numsubsecentry = \numsecentry \let\appsubsecentry = \numsecentry \let\unnsubsecentry = \numsecentry \let\numsubsubsecentry = \numsecentry \let\appsubsubsecentry = \numsecentry \let\unnsubsubsecentry = \numsecentry \openin 1 \tocreadfilename\space \ifeof 1 \else \readtocfile \fi \closein 1 \vfill \eject \contentsalignmacro % in case @setchapternewpage odd is in effect \endgroup \lastnegativepageno = \pageno \global\pageno = \savepageno } \let\shortcontents = \summarycontents % Typeset the label for a chapter or appendix for the short contents. % The arg is, e.g., `A' for an appendix, or `3' for a chapter. % \def\shortchaplabel#1{% % This space should be enough, since a single number is .5em, and the % widest letter (M) is 1em, at least in the Computer Modern fonts. % But use \hss just in case. % (This space doesn't include the extra space that gets added after % the label; that gets put in by \shortchapentry above.) % % We'd like to right-justify chapter numbers, but that looks strange % with appendix letters. And right-justifying numbers and % left-justifying letters looks strange when there is less than 10 % chapters. Have to read the whole toc once to know how many chapters % there are before deciding ... \hbox to 1em{#1\hss}% } % These macros generate individual entries in the table of contents. % The first argument is the chapter or section name. % The last argument is the page number. % The arguments in between are the chapter number, section number, ... % Parts, in the main contents. Replace the part number, which doesn't % exist, with an empty box. Let's hope all the numbers have the same width. % Also ignore the page number, which is conventionally not printed. \def\numeralbox{\setbox0=\hbox{8}\hbox to \wd0{\hfil}} \def\partentry#1#2#3#4{\dochapentry{\numeralbox\labelspace#1}{}} % % Parts, in the short toc. \def\shortpartentry#1#2#3#4{% \penalty-300 \vskip.5\baselineskip plus.15\baselineskip minus.1\baselineskip \shortchapentry{{\bf #1}}{\numeralbox}{}{}% } % Chapters, in the main contents. \def\numchapentry#1#2#3#4{\dochapentry{#2\labelspace#1}{#4}} % Chapters, in the short toc. % See comments in \dochapentry re vbox and related settings. \def\shortchapentry#1#2#3#4{% \tocentry{\shortchaplabel{#2}\labelspace #1}{\doshortpageno\bgroup#4\egroup}% } % Appendices, in the main contents. % Need the word Appendix, and a fixed-size box. % \def\appendixbox#1{% % We use M since it's probably the widest letter. \setbox0 = \hbox{\putwordAppendix{} M}% \hbox to \wd0{\putwordAppendix{} #1\hss}} % \def\appentry#1#2#3#4{\dochapentry{\appendixbox{#2}\hskip.7em#1}{#4}} % Unnumbered chapters. \def\unnchapentry#1#2#3#4{\dochapentry{#1}{#4}} \def\shortunnchapentry#1#2#3#4{\tocentry{#1}{\doshortpageno\bgroup#4\egroup}} % Sections. \def\numsecentry#1#2#3#4{\dosecentry{#2\labelspace#1}{#4}} \let\appsecentry=\numsecentry \def\unnsecentry#1#2#3#4{\dosecentry{#1}{#4}} % Subsections. \def\numsubsecentry#1#2#3#4{\dosubsecentry{#2\labelspace#1}{#4}} \let\appsubsecentry=\numsubsecentry \def\unnsubsecentry#1#2#3#4{\dosubsecentry{#1}{#4}} % And subsubsections. \def\numsubsubsecentry#1#2#3#4{\dosubsubsecentry{#2\labelspace#1}{#4}} \let\appsubsubsecentry=\numsubsubsecentry \def\unnsubsubsecentry#1#2#3#4{\dosubsubsecentry{#1}{#4}} % This parameter controls the indentation of the various levels. % Same as \defaultparindent. \newdimen\tocindent \tocindent = 15pt % Now for the actual typesetting. In all these, #1 is the text and #2 is the % page number. % % If the toc has to be broken over pages, we want it to be at chapters % if at all possible; hence the \penalty. \def\dochapentry#1#2{% \penalty-300 \vskip1\baselineskip plus.33\baselineskip minus.25\baselineskip \begingroup % Move the page numbers slightly to the right \advance\entryrightmargin by -0.05em \chapentryfonts \tocentry{#1}{\dopageno\bgroup#2\egroup}% \endgroup \nobreak\vskip .25\baselineskip plus.1\baselineskip } \def\dosecentry#1#2{\begingroup \secentryfonts \leftskip=\tocindent \tocentry{#1}{\dopageno\bgroup#2\egroup}% \endgroup} \def\dosubsecentry#1#2{\begingroup \subsecentryfonts \leftskip=2\tocindent \tocentry{#1}{\dopageno\bgroup#2\egroup}% \endgroup} \def\dosubsubsecentry#1#2{\begingroup \subsubsecentryfonts \leftskip=3\tocindent \tocentry{#1}{\dopageno\bgroup#2\egroup}% \endgroup} % We use the same \entry macro as for the index entries. \let\tocentry = \entry % Space between chapter (or whatever) number and the title. \def\labelspace{\hskip1em \relax} \def\dopageno#1{{\rm #1}} \def\doshortpageno#1{{\rm #1}} \def\chapentryfonts{\secfonts \rm} \def\secentryfonts{\textfonts} \def\subsecentryfonts{\textfonts} \def\subsubsecentryfonts{\textfonts} \message{environments,} % @foo ... @end foo. % @tex ... @end tex escapes into raw TeX temporarily. % One exception: @ is still an escape character, so that @end tex works. % But \@ or @@ will get a plain @ character. \envdef\tex{% \setupmarkupstyle{tex}% \catcode `\\=0 \catcode `\{=1 \catcode `\}=2 \catcode `\$=3 \catcode `\&=4 \catcode `\#=6 \catcode `\^=7 \catcode `\_=8 \catcode `\~=\active \let~=\tie \catcode `\%=14 \catcode `\+=\other \catcode `\"=\other \catcode `\|=\other \catcode `\<=\other \catcode `\>=\other \catcode `\`=\other \catcode `\'=\other % % ' is active in math mode (mathcode"8000). So reset it, and all our % other math active characters (just in case), to plain's definitions. \mathactive % % Inverse of the list at the beginning of the file. \let\b=\ptexb \let\bullet=\ptexbullet \let\c=\ptexc \let\,=\ptexcomma \let\.=\ptexdot \let\dots=\ptexdots \let\equiv=\ptexequiv \let\!=\ptexexclam \let\i=\ptexi \let\indent=\ptexindent \let\noindent=\ptexnoindent \let\{=\ptexlbrace \let\+=\tabalign \let\}=\ptexrbrace \let\/=\ptexslash \let\sp=\ptexsp \let\*=\ptexstar %\let\sup=\ptexsup % do not redefine, we want @sup to work in math mode \let\t=\ptext \expandafter \let\csname top\endcsname=\ptextop % we've made it outer \let\frenchspacing=\plainfrenchspacing % \def\endldots{\mathinner{\ldots\ldots\ldots\ldots}}% \def\enddots{\relax\ifmmode\endldots\else$\mathsurround=0pt \endldots\,$\fi}% \def\@{@}% } % There is no need to define \Etex. % Define @lisp ... @end lisp. % @lisp environment forms a group so it can rebind things, % including the definition of @end lisp (which normally is erroneous). % Amount to narrow the margins by for @lisp. \newskip\lispnarrowing \lispnarrowing=0.4in % This is the definition that ^^M gets inside @lisp, @example, and other % such environments. \null is better than a space, since it doesn't % have any width. \def\lisppar{\null\endgraf} % This space is always present above and below environments. \newskip\envskipamount \envskipamount = 0pt % Make spacing and below environment symmetrical. We use \parskip here % to help in doing that, since in @example-like environments \parskip % is reset to zero; thus the \afterenvbreak inserts no space -- but the % start of the next paragraph will insert \parskip. % \def\aboveenvbreak{{% % =10000 instead of <10000 because of a special case in \itemzzz and % \sectionheading, q.v. \ifnum \lastpenalty=10000 \else \advance\envskipamount by \parskip \endgraf \ifdim\lastskip<\envskipamount \removelastskip \ifnum\lastpenalty<10000 % Penalize breaking before the environment, because preceding text % often leads into it. \penalty100 \fi \vskip\envskipamount \fi \fi }} \def\afterenvbreak{{% % =10000 instead of <10000 because of a special case in \itemzzz and % \sectionheading, q.v. \ifnum \lastpenalty=10000 \else \advance\envskipamount by \parskip \endgraf \ifdim\lastskip<\envskipamount \removelastskip % it's not a good place to break if the last penalty was \nobreak % or better ... \ifnum\lastpenalty<10000 \penalty-50 \fi \vskip\envskipamount \fi \fi }} % \nonarrowing is a flag. If "set", @lisp etc don't narrow margins; it will % also clear it, so that its embedded environments do the narrowing again. \let\nonarrowing=\relax % @cartouche ... @end cartouche: draw rectangle w/rounded corners around % environment contents. \font\circle=lcircle10 \newdimen\circthick \newdimen\cartouter\newdimen\cartinner \newskip\normbskip\newskip\normpskip\newskip\normlskip \circthick=\fontdimen8\circle % \def\ctl{{\circle\char'013\hskip -6pt}}% 6pt from pl file: 1/2charwidth \def\ctr{{\hskip 6pt\circle\char'010}} \def\cbl{{\circle\char'012\hskip -6pt}} \def\cbr{{\hskip 6pt\circle\char'011}} \def\carttop{\hbox to \cartouter{\hskip\lskip \ctl\leaders\hrule height\circthick\hfil\ctr \hskip\rskip}} \def\cartbot{\hbox to \cartouter{\hskip\lskip \cbl\leaders\hrule height\circthick\hfil\cbr \hskip\rskip}} % \newskip\lskip\newskip\rskip \envdef\cartouche{% \ifhmode\par\fi % can't be in the midst of a paragraph. \startsavinginserts \lskip=\leftskip \rskip=\rightskip \leftskip=0pt\rightskip=0pt % we want these *outside*. \cartinner=\hsize \advance\cartinner by-\lskip \advance\cartinner by-\rskip \cartouter=\hsize \advance\cartouter by 18.4pt % allow for 3pt kerns on either % side, and for 6pt waste from % each corner char, and rule thickness \normbskip=\baselineskip \normpskip=\parskip \normlskip=\lineskip % % If this cartouche directly follows a sectioning command, we need the % \parskip glue (backspaced over by default) or the cartouche can % collide with the section heading. \ifnum\lastpenalty>10000 \vskip\parskip \penalty\lastpenalty \fi % \setbox\groupbox=\vbox\bgroup \baselineskip=0pt\parskip=0pt\lineskip=0pt \carttop \hbox\bgroup \hskip\lskip \vrule\kern3pt \vbox\bgroup \kern3pt \hsize=\cartinner \baselineskip=\normbskip \lineskip=\normlskip \parskip=\normpskip \vskip -\parskip \comment % For explanation, see the end of def\group. } \def\Ecartouche{% \ifhmode\par\fi \kern3pt \egroup \kern3pt\vrule \hskip\rskip \egroup \cartbot \egroup \addgroupbox \checkinserts } % This macro is called at the beginning of all the @example variants, % inside a group. \newdimen\nonfillparindent \def\nonfillstart{% \aboveenvbreak \ifdim\hfuzz < 12pt \hfuzz = 12pt \fi % Don't be fussy \sepspaces % Make spaces be word-separators rather than space tokens. \let\par = \lisppar % don't ignore blank lines \obeylines % each line of input is a line of output \parskip = 0pt % Turn off paragraph indentation but redefine \indent to emulate % the normal \indent. \nonfillparindent=\parindent \parindent = 0pt \let\indent\nonfillindent % \emergencystretch = 0pt % don't try to avoid overfull boxes \ifx\nonarrowing\relax \advance \leftskip by \lispnarrowing \exdentamount=\lispnarrowing \else \let\nonarrowing = \relax \fi \let\exdent=\nofillexdent } \begingroup \obeyspaces % We want to swallow spaces (but not other tokens) after the fake % @indent in our nonfill-environments, where spaces are normally % active and set to @tie, resulting in them not being ignored after % @indent. \gdef\nonfillindent{\futurelet\temp\nonfillindentcheck}% \gdef\nonfillindentcheck{% \ifx\temp % \expandafter\nonfillindentgobble% \else% \leavevmode\nonfillindentbox% \fi% }% \endgroup \def\nonfillindentgobble#1{\nonfillindent} \def\nonfillindentbox{\hbox to \nonfillparindent{\hss}} % If you want all examples etc. small: @set dispenvsize small. % If you want even small examples the full size: @set dispenvsize nosmall. % This affects the following displayed environments: % @example, @display, @format, @lisp % \def\smallword{small} \def\nosmallword{nosmall} \let\SETdispenvsize\relax \def\setnormaldispenv{% \ifx\SETdispenvsize\smallword % end paragraph for sake of leading, in case document has no blank % line. This is redundant with what happens in \aboveenvbreak, but % we need to do it before changing the fonts, and it's inconvenient % to change the fonts afterward. \ifnum \lastpenalty=10000 \else \endgraf \fi \smallexamplefonts \rm \fi } \def\setsmalldispenv{% \ifx\SETdispenvsize\nosmallword \else \ifnum \lastpenalty=10000 \else \endgraf \fi \smallexamplefonts \rm \fi } % We often define two environments, @foo and @smallfoo. % Let's do it in one command. #1 is the env name, #2 the definition. \def\makedispenvdef#1#2{% \expandafter\envdef\csname#1\endcsname {\setnormaldispenv #2}% \expandafter\envdef\csname small#1\endcsname {\setsmalldispenv #2}% \expandafter\let\csname E#1\endcsname \afterenvbreak \expandafter\let\csname Esmall#1\endcsname \afterenvbreak } % Define two environment synonyms (#1 and #2) for an environment. \def\maketwodispenvdef#1#2#3{% \makedispenvdef{#1}{#3}% \makedispenvdef{#2}{#3}% } % % @lisp: indented, narrowed, typewriter font; % @example: same as @lisp. % % @smallexample and @smalllisp: use smaller fonts. % Originally contributed by Pavel@xerox. % \maketwodispenvdef{lisp}{example}{% \nonfillstart \tt\setupmarkupstyle{example}% \let\kbdfont = \kbdexamplefont % Allow @kbd to do something special. \gobble % eat return } % @display/@smalldisplay: same as @lisp except keep current font. % \makedispenvdef{display}{% \nonfillstart \gobble } % @format/@smallformat: same as @display except don't narrow margins. % \makedispenvdef{format}{% \let\nonarrowing = t% \nonfillstart \gobble } % @flushleft: same as @format, but doesn't obey \SETdispenvsize. \envdef\flushleft{% \let\nonarrowing = t% \nonfillstart \gobble } \let\Eflushleft = \afterenvbreak % @flushright. % \envdef\flushright{% \let\nonarrowing = t% \nonfillstart \advance\leftskip by 0pt plus 1fill\relax \gobble } \let\Eflushright = \afterenvbreak % @raggedright does more-or-less normal line breaking but no right % justification. From plain.tex. Don't stretch around special % characters in urls in this environment, since the stretch at the right % should be enough. \envdef\raggedright{% \rightskip0pt plus2.4em \spaceskip.3333em \xspaceskip.5em\relax \def\urefprestretchamount{0pt}% \def\urefpoststretchamount{0pt}% } \let\Eraggedright\par \envdef\raggedleft{% \parindent=0pt \leftskip0pt plus2em \spaceskip.3333em \xspaceskip.5em \parfillskip=0pt \hbadness=10000 % Last line will usually be underfull, so turn off % badness reporting. } \let\Eraggedleft\par \envdef\raggedcenter{% \parindent=0pt \rightskip0pt plus1em \leftskip0pt plus1em \spaceskip.3333em \xspaceskip.5em \parfillskip=0pt \hbadness=10000 % Last line will usually be underfull, so turn off % badness reporting. } \let\Eraggedcenter\par % @quotation does normal linebreaking (hence we can't use \nonfillstart) % and narrows the margins. We keep \parskip nonzero in general, since % we're doing normal filling. So, when using \aboveenvbreak and % \afterenvbreak, temporarily make \parskip 0. % \makedispenvdef{quotation}{\quotationstart} % \def\quotationstart{% \indentedblockstart % same as \indentedblock, but increase right margin too. \ifx\nonarrowing\relax \advance\rightskip by \lispnarrowing \fi \parsearg\quotationlabel } % We have retained a nonzero parskip for the environment, since we're % doing normal filling. % \def\Equotation{% \par \ifx\quotationauthor\thisisundefined\else % indent a bit. \leftline{\kern 2\leftskip \sl ---\quotationauthor}% \fi {\parskip=0pt \afterenvbreak}% } \def\Esmallquotation{\Equotation} % If we're given an argument, typeset it in bold with a colon after. \def\quotationlabel#1{% \def\temp{#1}% \ifx\temp\empty \else {\bf #1: }% \fi } % @indentedblock is like @quotation, but indents only on the left and % has no optional argument. % \makedispenvdef{indentedblock}{\indentedblockstart} % \def\indentedblockstart{% {\parskip=0pt \aboveenvbreak}% because \aboveenvbreak inserts \parskip \parindent=0pt % % @cartouche defines \nonarrowing to inhibit narrowing at next level down. \ifx\nonarrowing\relax \advance\leftskip by \lispnarrowing \exdentamount = \lispnarrowing \else \let\nonarrowing = \relax \fi } % Keep a nonzero parskip for the environment, since we're doing normal filling. % \def\Eindentedblock{% \par {\parskip=0pt \afterenvbreak}% } \def\Esmallindentedblock{\Eindentedblock} % LaTeX-like @verbatim...@end verbatim and @verb{<char>...<char>} % If we want to allow any <char> as delimiter, % we need the curly braces so that makeinfo sees the @verb command, eg: % `@verbx...x' would look like the '@verbx' command. --janneke@gnu.org % % [Knuth]: Donald Ervin Knuth, 1996. The TeXbook. % % [Knuth] p.344; only we need to do the other characters Texinfo sets % active too. Otherwise, they get lost as the first character on a % verbatim line. \def\dospecials{% \do\ \do\\\do\{\do\}\do\$\do\&% \do\#\do\^\do\^^K\do\_\do\^^A\do\%\do\~% \do\<\do\>\do\|\do\@\do+\do\"% % Don't do the quotes -- if we do, @set txicodequoteundirected and % @set txicodequotebacktick will not have effect on @verb and % @verbatim, and ?` and !` ligatures won't get disabled. %\do\`\do\'% } % % [Knuth] p. 380 \def\uncatcodespecials{% \def\do##1{\catcode`##1=\other}\dospecials} % % Setup for the @verb command. % % Eight spaces for a tab \begingroup \catcode`\^^I=\active \gdef\tabeightspaces{\catcode`\^^I=\active\def^^I{\ \ \ \ \ \ \ \ }} \endgroup % \def\setupverb{% \tt % easiest (and conventionally used) font for verbatim \def\par{\leavevmode\endgraf}% \setupmarkupstyle{verb}% \tabeightspaces % Respect line breaks, % print special symbols as themselves, and % make each space count % must do in this order: \obeylines \uncatcodespecials \sepspaces } % Setup for the @verbatim environment % % Real tab expansion. \newdimen\tabw \setbox0=\hbox{\tt\space} \tabw=8\wd0 % tab amount % % We typeset each line of the verbatim in an \hbox, so we can handle % tabs. The \global is in case the verbatim line starts with an accent, % or some other command that starts with a begin-group. Otherwise, the % entire \verbbox would disappear at the corresponding end-group, before % it is typeset. Meanwhile, we can't have nested verbatim commands % (can we?), so the \global won't be overwriting itself. \newbox\verbbox \def\starttabbox{\global\setbox\verbbox=\hbox\bgroup} % \begingroup \catcode`\^^I=\active \gdef\tabexpand{% \catcode`\^^I=\active \def^^I{\leavevmode\egroup \dimen\verbbox=\wd\verbbox % the width so far, or since the previous tab \divide\dimen\verbbox by\tabw \multiply\dimen\verbbox by\tabw % compute previous multiple of \tabw \advance\dimen\verbbox by\tabw % advance to next multiple of \tabw \wd\verbbox=\dimen\verbbox \box\verbbox \starttabbox }% } \endgroup % start the verbatim environment. \def\setupverbatim{% \let\nonarrowing = t% \nonfillstart \tt % easiest (and conventionally used) font for verbatim % The \leavevmode here is for blank lines. Otherwise, we would % never \starttabox and the \egroup would end verbatim mode. \def\par{\leavevmode\egroup\box\verbbox\endgraf}% \tabexpand \setupmarkupstyle{verbatim}% % Respect line breaks, % print special symbols as themselves, and % make each space count. % Must do in this order: \obeylines \uncatcodespecials \sepspaces \everypar{\starttabbox}% } % Do the @verb magic: verbatim text is quoted by unique % delimiter characters. Before first delimiter expect a % right brace, after last delimiter expect closing brace: % % \def\doverb'{'<char>#1<char>'}'{#1} % % [Knuth] p. 382; only eat outer {} \begingroup \catcode`[=1\catcode`]=2\catcode`\{=\other\catcode`\}=\other \gdef\doverb{#1[\def\next##1#1}[##1\endgroup]\next] \endgroup % \def\verb{\begingroup\setupverb\doverb} % % % Do the @verbatim magic: define the macro \doverbatim so that % the (first) argument ends when '@end verbatim' is reached, ie: % % \def\doverbatim#1@end verbatim{#1} % % For Texinfo it's a lot easier than for LaTeX, % because texinfo's \verbatim doesn't stop at '\end{verbatim}': % we need not redefine '\', '{' and '}'. % % Inspired by LaTeX's verbatim command set [latex.ltx] % \begingroup \catcode`\ =\active \obeylines % % ignore everything up to the first ^^M, that's the newline at the end % of the @verbatim input line itself. Otherwise we get an extra blank % line in the output. \xdef\doverbatim#1^^M#2@end verbatim{#2\noexpand\end\gobble verbatim}% % We really want {...\end verbatim} in the body of the macro, but % without the active space; thus we have to use \xdef and \gobble. \endgroup % \envdef\verbatim{% \setupverbatim\doverbatim } \let\Everbatim = \afterenvbreak % @verbatiminclude FILE - insert text of file in verbatim environment. % \def\verbatiminclude{\parseargusing\filenamecatcodes\doverbatiminclude} % \def\doverbatiminclude#1{% {% \makevalueexpandable \setupverbatim \indexnofonts % Allow `@@' and other weird things in file names. \wlog{texinfo.tex: doing @verbatiminclude of #1^^J}% \input #1 \afterenvbreak }% } % @copying ... @end copying. % Save the text away for @insertcopying later. % % We save the uninterpreted tokens, rather than creating a box. % Saving the text in a box would be much easier, but then all the % typesetting commands (@smallbook, font changes, etc.) have to be done % beforehand -- and a) we want @copying to be done first in the source % file; b) letting users define the frontmatter in as flexible order as % possible is desirable. % \def\copying{\checkenv{}\begingroup\scanargctxt\docopying} \def\docopying#1@end copying{\endgroup\def\copyingtext{#1}} % \def\insertcopying{% \begingroup \parindent = 0pt % paragraph indentation looks wrong on title page \scanexp\copyingtext \endgroup } \message{defuns,} % @defun etc. \newskip\defbodyindent \defbodyindent=.4in \newskip\defargsindent \defargsindent=50pt \newskip\deflastargmargin \deflastargmargin=18pt \newcount\defunpenalty % Start the processing of @deffn: \def\startdefun{% \ifnum\lastpenalty<10000 \medbreak \defunpenalty=10003 % Will keep this @deffn together with the % following @def command, see below. \else % If there are two @def commands in a row, we'll have a \nobreak, % which is there to keep the function description together with its % header. But if there's nothing but headers, we need to allow a % break somewhere. Check specifically for penalty 10002, inserted % by \printdefunline, instead of 10000, since the sectioning % commands also insert a nobreak penalty, and we don't want to allow % a break between a section heading and a defun. % % As a further refinement, we avoid "club" headers by signalling % with penalty of 10003 after the very first @deffn in the % sequence (see above), and penalty of 10002 after any following % @def command. \ifnum\lastpenalty=10002 \penalty2000 \else \defunpenalty=10002 \fi % % Similarly, after a section heading, do not allow a break. % But do insert the glue. \medskip % preceded by discardable penalty, so not a breakpoint \fi % \parindent=0in \advance\leftskip by \defbodyindent \exdentamount=\defbodyindent } \def\dodefunx#1{% % First, check whether we are in the right environment: \checkenv#1% % % As above, allow line break if we have multiple x headers in a row. % It's not a great place, though. \ifnum\lastpenalty=10002 \penalty3000 \else \defunpenalty=10002 \fi % % And now, it's time to reuse the body of the original defun: \expandafter\gobbledefun#1% } \def\gobbledefun#1\startdefun{} % \printdefunline \deffnheader{text} % \def\printdefunline#1#2{% \begingroup % call \deffnheader: #1#2 \endheader % common ending: \interlinepenalty = 10000 \advance\rightskip by 0pt plus 1fil\relax \endgraf \nobreak\vskip -\parskip \penalty\defunpenalty % signal to \startdefun and \dodefunx % Some of the @defun-type tags do not enable magic parentheses, % rendering the following check redundant. But we don't optimize. \checkparencounts \endgroup } \def\Edefun{\endgraf\medbreak} % \makedefun{deffn} creates \deffn, \deffnx and \Edeffn; % the only thing remaining is to define \deffnheader. % \def\makedefun#1{% \expandafter\let\csname E#1\endcsname = \Edefun \edef\temp{\noexpand\domakedefun \makecsname{#1}\makecsname{#1x}\makecsname{#1header}}% \temp } % \domakedefun \deffn \deffnx \deffnheader { (defn. of \deffnheader) } % % Define \deffn and \deffnx, without parameters. % \deffnheader has to be defined explicitly. % \def\domakedefun#1#2#3{% \envdef#1{% \startdefun \doingtypefnfalse % distinguish typed functions from all else \parseargusing\activeparens{\printdefunline#3}% }% \def#2{\dodefunx#1}% \def#3% } \newif\ifdoingtypefn % doing typed function? \newif\ifrettypeownline % typeset return type on its own line? % @deftypefnnewline on|off says whether the return type of typed functions % are printed on their own line. This affects @deftypefn, @deftypefun, % @deftypeop, and @deftypemethod. % \parseargdef\deftypefnnewline{% \def\temp{#1}% \ifx\temp\onword \expandafter\let\csname SETtxideftypefnnl\endcsname = \empty \else\ifx\temp\offword \expandafter\let\csname SETtxideftypefnnl\endcsname = \relax \else \errhelp = \EMsimple \errmessage{Unknown @txideftypefnnl value `\temp', must be on|off}% \fi\fi } % Untyped functions: % @deffn category name args \makedefun{deffn}{\deffngeneral{}} % @deffn category class name args \makedefun{defop}#1 {\defopon{#1\ \putwordon}} % \defopon {category on}class name args \def\defopon#1#2 {\deffngeneral{\putwordon\ \code{#2}}{#1\ \code{#2}} } % \deffngeneral {subind}category name args % \def\deffngeneral#1#2 #3 #4\endheader{% % Remember that \dosubind{fn}{foo}{} is equivalent to \doind{fn}{foo}. \dosubind{fn}{\code{#3}}{#1}% \defname{#2}{}{#3}\magicamp\defunargs{#4\unskip}% } % Typed functions: % @deftypefn category type name args \makedefun{deftypefn}{\deftypefngeneral{}} % @deftypeop category class type name args \makedefun{deftypeop}#1 {\deftypeopon{#1\ \putwordon}} % \deftypeopon {category on}class type name args \def\deftypeopon#1#2 {\deftypefngeneral{\putwordon\ \code{#2}}{#1\ \code{#2}} } % \deftypefngeneral {subind}category type name args % \def\deftypefngeneral#1#2 #3 #4 #5\endheader{% \dosubind{fn}{\code{#4}}{#1}% \doingtypefntrue \defname{#2}{#3}{#4}\defunargs{#5\unskip}% } % Typed variables: % @deftypevr category type var args \makedefun{deftypevr}{\deftypecvgeneral{}} % @deftypecv category class type var args \makedefun{deftypecv}#1 {\deftypecvof{#1\ \putwordof}} % \deftypecvof {category of}class type var args \def\deftypecvof#1#2 {\deftypecvgeneral{\putwordof\ \code{#2}}{#1\ \code{#2}} } % \deftypecvgeneral {subind}category type var args % \def\deftypecvgeneral#1#2 #3 #4 #5\endheader{% \dosubind{vr}{\code{#4}}{#1}% \defname{#2}{#3}{#4}\defunargs{#5\unskip}% } % Untyped variables: % @defvr category var args \makedefun{defvr}#1 {\deftypevrheader{#1} {} } % @defcv category class var args \makedefun{defcv}#1 {\defcvof{#1\ \putwordof}} % \defcvof {category of}class var args \def\defcvof#1#2 {\deftypecvof{#1}#2 {} } % Types: % @deftp category name args \makedefun{deftp}#1 #2 #3\endheader{% \doind{tp}{\code{#2}}% \defname{#1}{}{#2}\defunargs{#3\unskip}% } % Remaining @defun-like shortcuts: \makedefun{defun}{\deffnheader{\putwordDeffunc} } \makedefun{defmac}{\deffnheader{\putwordDefmac} } \makedefun{defspec}{\deffnheader{\putwordDefspec} } \makedefun{deftypefun}{\deftypefnheader{\putwordDeffunc} } \makedefun{defvar}{\defvrheader{\putwordDefvar} } \makedefun{defopt}{\defvrheader{\putwordDefopt} } \makedefun{deftypevar}{\deftypevrheader{\putwordDefvar} } \makedefun{defmethod}{\defopon\putwordMethodon} \makedefun{deftypemethod}{\deftypeopon\putwordMethodon} \makedefun{defivar}{\defcvof\putwordInstanceVariableof} \makedefun{deftypeivar}{\deftypecvof\putwordInstanceVariableof} % \defname, which formats the name of the @def (not the args). % #1 is the category, such as "Function". % #2 is the return type, if any. % #3 is the function name. % % We are followed by (but not passed) the arguments, if any. % \def\defname#1#2#3{% \par % Get the values of \leftskip and \rightskip as they were outside the @def... \advance\leftskip by -\defbodyindent % % Determine if we are typesetting the return type of a typed function % on a line by itself. \rettypeownlinefalse \ifdoingtypefn % doing a typed function specifically? % then check user option for putting return type on its own line: \expandafter\ifx\csname SETtxideftypefnnl\endcsname\relax \else \rettypeownlinetrue \fi \fi % % How we'll format the category name. Putting it in brackets helps % distinguish it from the body text that may end up on the next line % just below it. \def\temp{#1}% \setbox0=\hbox{\kern\deflastargmargin \ifx\temp\empty\else [\rm\temp]\fi} % % Figure out line sizes for the paragraph shape. We'll always have at % least two. \tempnum = 2 % % The first line needs space for \box0; but if \rightskip is nonzero, % we need only space for the part of \box0 which exceeds it: \dimen0=\hsize \advance\dimen0 by -\wd0 \advance\dimen0 by \rightskip % % If doing a return type on its own line, we'll have another line. \ifrettypeownline \advance\tempnum by 1 \def\maybeshapeline{0in \hsize}% \else \def\maybeshapeline{}% \fi % % The continuations: \dimen2=\hsize \advance\dimen2 by -\defargsindent % % The final paragraph shape: \parshape \tempnum 0in \dimen0 \maybeshapeline \defargsindent \dimen2 % % Put the category name at the right margin. \noindent \hbox to 0pt{% \hfil\box0 \kern-\hsize % \hsize has to be shortened this way: \kern\leftskip % Intentionally do not respect \rightskip, since we need the space. }% % % Allow all lines to be underfull without complaint: \tolerance=10000 \hbadness=10000 \exdentamount=\defbodyindent {% % defun fonts. We use typewriter by default (used to be bold) because: % . we're printing identifiers, they should be in tt in principle. % . in languages with many accents, such as Czech or French, it's % common to leave accents off identifiers. The result looks ok in % tt, but exceedingly strange in rm. % . we don't want -- and --- to be treated as ligatures. % . this still does not fix the ?` and !` ligatures, but so far no % one has made identifiers using them :). \df \tt \def\temp{#2}% text of the return type \ifx\temp\empty\else \tclose{\temp}% typeset the return type \ifrettypeownline % put return type on its own line; prohibit line break following: \hfil\vadjust{\nobreak}\break \else \space % type on same line, so just followed by a space \fi \fi % no return type #3% output function name }% {\rm\enskip}% hskip 0.5 em of \rmfont % \boldbrax % arguments will be output next, if any. } % Print arguments in slanted roman (not ttsl), inconsistently with using % tt for the name. This is because literal text is sometimes needed in % the argument list (groff manual), and ttsl and tt are not very % distinguishable. Prevent hyphenation at `-' chars. % \def\defunargs#1{% % use sl by default (not ttsl), % tt for the names. \df \sl \hyphenchar\font=0 % % On the other hand, if an argument has two dashes (for instance), we % want a way to get ttsl. We used to recommend @var for that, so % leave the code in, but it's strange for @var to lead to typewriter. % Nowadays we recommend @code, since the difference between a ttsl hyphen % and a tt hyphen is pretty tiny. @code also disables ?` !`. \def\var##1{{\setupmarkupstyle{var}\ttslanted{##1}}}% #1% \sl\hyphenchar\font=45 } % We want ()&[] to print specially on the defun line. % \def\activeparens{% \catcode`\(=\active \catcode`\)=\active \catcode`\[=\active \catcode`\]=\active \catcode`\&=\active } % Make control sequences which act like normal parenthesis chars. \let\lparen = ( \let\rparen = ) % Be sure that we always have a definition for `(', etc. For example, % if the fn name has parens in it, \boldbrax will not be in effect yet, % so TeX would otherwise complain about undefined control sequence. { \activeparens \global\let(=\lparen \global\let)=\rparen \global\let[=\lbrack \global\let]=\rbrack \global\let& = \& \gdef\boldbrax{\let(=\opnr\let)=\clnr\let[=\lbrb\let]=\rbrb} \gdef\magicamp{\let&=\amprm} } \newcount\parencount % If we encounter &foo, then turn on ()-hacking afterwards \newif\ifampseen \def\amprm#1 {\ampseentrue{\bf\ }} \def\parenfont{% \ifampseen % At the first level, print parens in roman, % otherwise use the default font. \ifnum \parencount=1 \rm \fi \else % The \sf parens (in \boldbrax) actually are a little bolder than % the contained text. This is especially needed for [ and ] . \sf \fi } \def\infirstlevel#1{% \ifampseen \ifnum\parencount=1 #1% \fi \fi } \def\bfafterword#1 {#1 \bf} \def\opnr{% \global\advance\parencount by 1 {\parenfont(}% \infirstlevel \bfafterword } \def\clnr{% {\parenfont)}% \infirstlevel \sl \global\advance\parencount by -1 } \newcount\brackcount \def\lbrb{% \global\advance\brackcount by 1 {\bf[}% } \def\rbrb{% {\bf]}% \global\advance\brackcount by -1 } \def\checkparencounts{% \ifnum\parencount=0 \else \badparencount \fi \ifnum\brackcount=0 \else \badbrackcount \fi } % these should not use \errmessage; the glibc manual, at least, actually % has such constructs (when documenting function pointers). \def\badparencount{% \message{Warning: unbalanced parentheses in @def...}% \global\parencount=0 } \def\badbrackcount{% \message{Warning: unbalanced square brackets in @def...}% \global\brackcount=0 } \message{macros,} % @macro. % To do this right we need a feature of e-TeX, \scantokens, % which we arrange to emulate with a temporary file in ordinary TeX. \ifx\eTeXversion\thisisundefined \newwrite\macscribble \def\scantokens#1{% \toks0={#1}% \immediate\openout\macscribble=\jobname.tmp \immediate\write\macscribble{\the\toks0}% \immediate\closeout\macscribble \input \jobname.tmp } \fi \let\aftermacroxxx\relax \def\aftermacro{\aftermacroxxx} % alias because \c means cedilla in @tex or @math \let\texinfoc=\c \newcount\savedcatcodeone \newcount\savedcatcodetwo % Used at the time of macro expansion. % Argument is macro body with arguments substituted \def\scanmacro#1{% \newlinechar`\^^M \def\xeatspaces{\eatspaces}% % % Temporarily undo catcode changes of \printindex. Set catcode of @ to % 0 so that @-commands in macro expansions aren't printed literally when % formatting an index file, where \ is used as the escape character. \savedcatcodeone=\catcode`\@ \savedcatcodetwo=\catcode`\\ \catcode`\@=0 \catcode`\\=\active % % Process the macro body under the current catcode regime. \scantokens{#1@texinfoc}\aftermacro% % \catcode`\@=\savedcatcodeone \catcode`\\=\savedcatcodetwo % % The \texinfoc is to remove the \newlinechar added by \scantokens, and % can be noticed by \parsearg. % The \aftermacro allows a \comment at the end of the macro definition % to duplicate itself past the final \newlinechar added by \scantokens: % this is used in the definition of \group to comment out a newline. We % don't do the same for \c to support Texinfo files with macros that ended % with a @c, which should no longer be necessary. % We avoid surrounding the call to \scantokens with \bgroup and \egroup % to allow macros to open or close groups themselves. } % Used for copying and captions \def\scanexp#1{% \expandafter\scanmacro\expandafter{#1}% } \newcount\paramno % Count of parameters \newtoks\macname % Macro name \newif\ifrecursive % Is it recursive? % List of all defined macros in the form % \commondummyword\macro1\commondummyword\macro2... % Currently is also contains all @aliases; the list can be split % if there is a need. \def\macrolist{} % Add the macro to \macrolist \def\addtomacrolist#1{\expandafter \addtomacrolistxxx \csname#1\endcsname} \def\addtomacrolistxxx#1{% \toks0 = \expandafter{\macrolist\commondummyword#1}% \xdef\macrolist{\the\toks0}% } % Utility routines. % This does \let #1 = #2, with \csnames; that is, % \let \csname#1\endcsname = \csname#2\endcsname % (except of course we have to play expansion games). % \def\cslet#1#2{% \expandafter\let \csname#1\expandafter\endcsname \csname#2\endcsname } % Trim leading and trailing spaces off a string. % Concepts from aro-bend problem 15 (see CTAN). {\catcode`\@=11 \gdef\eatspaces #1{\expandafter\trim@\expandafter{#1 }} \gdef\trim@ #1{\trim@@ @#1 @ #1 @ @@} \gdef\trim@@ #1@ #2@ #3@@{\trim@@@\empty #2 @} \def\unbrace#1{#1} \unbrace{\gdef\trim@@@ #1 } #2@{#1} } % Trim a single trailing ^^M off a string. {\catcode`\^^M=\other \catcode`\Q=3% \gdef\eatcr #1{\eatcra #1Q^^MQ}% \gdef\eatcra#1^^MQ{\eatcrb#1Q}% \gdef\eatcrb#1Q#2Q{#1}% } % Macro bodies are absorbed as an argument in a context where % all characters are catcode 10, 11 or 12, except \ which is active % (as in normal texinfo). It is necessary to change the definition of \ % to recognize macro arguments; this is the job of \mbodybackslash. % % Non-ASCII encodings make 8-bit characters active, so un-activate % them to avoid their expansion. Must do this non-globally, to % confine the change to the current group. % % It's necessary to have hard CRs when the macro is executed. This is % done by making ^^M (\endlinechar) catcode 12 when reading the macro % body, and then making it the \newlinechar in \scanmacro. % \def\scanctxt{% used as subroutine \catcode`\"=\other \catcode`\+=\other \catcode`\<=\other \catcode`\>=\other \catcode`\^=\other \catcode`\_=\other \catcode`\|=\other \catcode`\~=\other \passthroughcharstrue } \def\scanargctxt{% used for copying and captions, not macros. \scanctxt \catcode`\@=\other \catcode`\\=\other \catcode`\^^M=\other } \def\macrobodyctxt{% used for @macro definitions \scanctxt \catcode`\ =\other \catcode`\@=\other \catcode`\{=\other \catcode`\}=\other \catcode`\^^M=\other \usembodybackslash } % Used when scanning braced macro arguments. Note, however, that catcode % changes here are ineffectual if the macro invocation was nested inside % an argument to another Texinfo command. \def\macroargctxt{% \scanctxt \catcode`\ =\active \catcode`\^^M=\other \catcode`\\=\active } \def\macrolineargctxt{% used for whole-line arguments without braces \scanctxt \catcode`\{=\other \catcode`\}=\other } % \mbodybackslash is the definition of \ in @macro bodies. % It maps \foo\ => \csname macarg.foo\endcsname => #N % where N is the macro parameter number. % We define \csname macarg.\endcsname to be \realbackslash, so % \\ in macro replacement text gets you a backslash. % {\catcode`@=0 @catcode`@\=@active @gdef@usembodybackslash{@let\=@mbodybackslash} @gdef@mbodybackslash#1\{@csname macarg.#1@endcsname} } \expandafter\def\csname macarg.\endcsname{\realbackslash} \def\margbackslash#1{\char`\#1 } \def\macro{\recursivefalse\parsearg\macroxxx} \def\rmacro{\recursivetrue\parsearg\macroxxx} \def\macroxxx#1{% \getargs{#1}% now \macname is the macname and \argl the arglist \ifx\argl\empty % no arguments \paramno=0\relax \else \expandafter\parsemargdef \argl;% \if\paramno>256\relax \ifx\eTeXversion\thisisundefined \errhelp = \EMsimple \errmessage{You need eTeX to compile a file with macros with more than 256 arguments} \fi \fi \fi \if1\csname ismacro.\the\macname\endcsname \message{Warning: redefining \the\macname}% \else \expandafter\ifx\csname \the\macname\endcsname \relax \else \errmessage{Macro name \the\macname\space already defined}\fi \global\cslet{macsave.\the\macname}{\the\macname}% \global\expandafter\let\csname ismacro.\the\macname\endcsname=1% \addtomacrolist{\the\macname}% \fi \begingroup \macrobodyctxt \ifrecursive \expandafter\parsermacbody \else \expandafter\parsemacbody \fi} \parseargdef\unmacro{% \if1\csname ismacro.#1\endcsname \global\cslet{#1}{macsave.#1}% \global\expandafter\let \csname ismacro.#1\endcsname=0% % Remove the macro name from \macrolist: \begingroup \expandafter\let\csname#1\endcsname \relax \let\commondummyword\unmacrodo \xdef\macrolist{\macrolist}% \endgroup \else \errmessage{Macro #1 not defined}% \fi } % Called by \do from \dounmacro on each macro. The idea is to omit any % macro definitions that have been changed to \relax. % \def\unmacrodo#1{% \ifx #1\relax % remove this \else \noexpand\commondummyword \noexpand#1% \fi } % \getargs -- Parse the arguments to a @macro line. Set \macname to % the name of the macro, and \argl to the braced argument list. \def\getargs#1{\getargsxxx#1{}} \def\getargsxxx#1#{\getmacname #1 \relax\getmacargs} \def\getmacname#1 #2\relax{\macname={#1}} \def\getmacargs#1{\def\argl{#1}} % This made use of the feature that if the last token of a % <parameter list> is #, then the preceding argument is delimited by % an opening brace, and that opening brace is not consumed. % Parse the optional {params} list to @macro or @rmacro. % Set \paramno to the number of arguments, % and \paramlist to a parameter text for the macro (e.g. #1,#2,#3 for a % three-param macro.) Define \macarg.BLAH for each BLAH in the params % list to some hook where the argument is to be expanded. If there are % less than 10 arguments that hook is to be replaced by ##N where N % is the position in that list, that is to say the macro arguments are to be % defined `a la TeX in the macro body. % % That gets used by \mbodybackslash (above). % % If there are 10 or more arguments, a different technique is used: see % \parsemmanyargdef. % \def\parsemargdef#1;{% \paramno=0\def\paramlist{}% \let\hash\relax % \hash is redefined to `#' later to get it into definitions \let\xeatspaces\relax \parsemargdefxxx#1,;,% \ifnum\paramno<10\relax\else \paramno0\relax \parsemmanyargdef@@#1,;,% 10 or more arguments \fi } \def\parsemargdefxxx#1,{% \if#1;\let\next=\relax \else \let\next=\parsemargdefxxx \advance\paramno by 1 \expandafter\edef\csname macarg.\eatspaces{#1}\endcsname {\xeatspaces{\hash\the\paramno}}% \edef\paramlist{\paramlist\hash\the\paramno,}% \fi\next} % \parsemacbody, \parsermacbody % % Read recursive and nonrecursive macro bodies. (They're different since % rec and nonrec macros end differently.) % % We are in \macrobodyctxt, and the \xdef causes backslashshes in the macro % body to be transformed. % Set \macrobody to the body of the macro, and call \defmacro. % {\catcode`\ =\other\long\gdef\parsemacbody#1@end macro{% \xdef\macrobody{\eatcr{#1}}\endgroup\defmacro}}% {\catcode`\ =\other\long\gdef\parsermacbody#1@end rmacro{% \xdef\macrobody{\eatcr{#1}}\endgroup\defmacro}}% % Make @ a letter, so that we can make private-to-Texinfo macro names. \edef\texiatcatcode{\the\catcode`\@} \catcode `@=11\relax %%%%%%%%%%%%%% Code for > 10 arguments only %%%%%%%%%%%%%%%%%% % If there are 10 or more arguments, a different technique is used, where the % hook remains in the body, and when macro is to be expanded the body is % processed again to replace the arguments. % % In that case, the hook is \the\toks N-1, and we simply set \toks N-1 to the % argument N value and then \edef the body (nothing else will expand because of % the catcode regime under which the body was input). % % If you compile with TeX (not eTeX), and you have macros with 10 or more % arguments, no macro can have more than 256 arguments (else error). % % In case that there are 10 or more arguments we parse again the arguments % list to set new definitions for the \macarg.BLAH macros corresponding to % each BLAH argument. It was anyhow needed to parse already once this list % in order to count the arguments, and as macros with at most 9 arguments % are by far more frequent than macro with 10 or more arguments, defining % twice the \macarg.BLAH macros does not cost too much processing power. \def\parsemmanyargdef@@#1,{% \if#1;\let\next=\relax \else \let\next=\parsemmanyargdef@@ \edef\tempb{\eatspaces{#1}}% \expandafter\def\expandafter\tempa \expandafter{\csname macarg.\tempb\endcsname}% % Note that we need some extra \noexpand\noexpand, this is because we % don't want \the to be expanded in the \parsermacbody as it uses an % \xdef . \expandafter\edef\tempa {\noexpand\noexpand\noexpand\the\toks\the\paramno}% \advance\paramno by 1\relax \fi\next} \let\endargs@\relax \let\nil@\relax \def\nilm@{\nil@}% \long\def\nillm@{\nil@}% % This macro is expanded during the Texinfo macro expansion, not during its % definition. It gets all the arguments' values and assigns them to macros % macarg.ARGNAME % % #1 is the macro name % #2 is the list of argument names % #3 is the list of argument values \def\getargvals@#1#2#3{% \def\macargdeflist@{}% \def\saveparamlist@{#2}% Need to keep a copy for parameter expansion. \def\paramlist{#2,\nil@}% \def\macroname{#1}% \begingroup \macroargctxt \def\argvaluelist{#3,\nil@}% \def\@tempa{#3}% \ifx\@tempa\empty \setemptyargvalues@ \else \getargvals@@ \fi } \def\getargvals@@{% \ifx\paramlist\nilm@ % Some sanity check needed here that \argvaluelist is also empty. \ifx\argvaluelist\nillm@ \else \errhelp = \EMsimple \errmessage{Too many arguments in macro `\macroname'!}% \fi \let\next\macargexpandinbody@ \else \ifx\argvaluelist\nillm@ % No more arguments values passed to macro. Set remaining named-arg % macros to empty. \let\next\setemptyargvalues@ \else % pop current arg name into \@tempb \def\@tempa##1{\pop@{\@tempb}{\paramlist}##1\endargs@}% \expandafter\@tempa\expandafter{\paramlist}% % pop current argument value into \@tempc \def\@tempa##1{\longpop@{\@tempc}{\argvaluelist}##1\endargs@}% \expandafter\@tempa\expandafter{\argvaluelist}% % Here \@tempb is the current arg name and \@tempc is the current arg value. % First place the new argument macro definition into \@tempd \expandafter\macname\expandafter{\@tempc}% \expandafter\let\csname macarg.\@tempb\endcsname\relax \expandafter\def\expandafter\@tempe\expandafter{% \csname macarg.\@tempb\endcsname}% \edef\@tempd{\long\def\@tempe{\the\macname}}% \push@\@tempd\macargdeflist@ \let\next\getargvals@@ \fi \fi \next } \def\push@#1#2{% \expandafter\expandafter\expandafter\def \expandafter\expandafter\expandafter#2% \expandafter\expandafter\expandafter{% \expandafter#1#2}% } % Replace arguments by their values in the macro body, and place the result % in macro \@tempa. % \def\macvalstoargs@{% % To do this we use the property that token registers that are \the'ed % within an \edef expand only once. So we are going to place all argument % values into respective token registers. % % First we save the token context, and initialize argument numbering. \begingroup \paramno0\relax % Then, for each argument number #N, we place the corresponding argument % value into a new token list register \toks#N \expandafter\putargsintokens@\saveparamlist@,;,% % Then, we expand the body so that argument are replaced by their % values. The trick for values not to be expanded themselves is that they % are within tokens and that tokens expand only once in an \edef . \edef\@tempc{\csname mac.\macroname .body\endcsname}% % Now we restore the token stack pointer to free the token list registers % which we have used, but we make sure that expanded body is saved after % group. \expandafter \endgroup \expandafter\def\expandafter\@tempa\expandafter{\@tempc}% } % Define the named-macro outside of this group and then close this group. % \def\macargexpandinbody@{% \expandafter \endgroup \macargdeflist@ % First the replace in body the macro arguments by their values, the result % is in \@tempa . \macvalstoargs@ % Then we point at the \norecurse or \gobble (for recursive) macro value % with \@tempb . \expandafter\let\expandafter\@tempb\csname mac.\macroname .recurse\endcsname % Depending on whether it is recursive or not, we need some tailing % \egroup . \ifx\@tempb\gobble \let\@tempc\relax \else \let\@tempc\egroup \fi % And now we do the real job: \edef\@tempd{\noexpand\@tempb{\macroname}\noexpand\scanmacro{\@tempa}\@tempc}% \@tempd } \def\putargsintokens@#1,{% \if#1;\let\next\relax \else \let\next\putargsintokens@ % First we allocate the new token list register, and give it a temporary % alias \@tempb . \toksdef\@tempb\the\paramno % Then we place the argument value into that token list register. \expandafter\let\expandafter\@tempa\csname macarg.#1\endcsname \expandafter\@tempb\expandafter{\@tempa}% \advance\paramno by 1\relax \fi \next } % Trailing missing arguments are set to empty. % \def\setemptyargvalues@{% \ifx\paramlist\nilm@ \let\next\macargexpandinbody@ \else \expandafter\setemptyargvaluesparser@\paramlist\endargs@ \let\next\setemptyargvalues@ \fi \next } \def\setemptyargvaluesparser@#1,#2\endargs@{% \expandafter\def\expandafter\@tempa\expandafter{% \expandafter\def\csname macarg.#1\endcsname{}}% \push@\@tempa\macargdeflist@ \def\paramlist{#2}% } % #1 is the element target macro % #2 is the list macro % #3,#4\endargs@ is the list value \def\pop@#1#2#3,#4\endargs@{% \def#1{#3}% \def#2{#4}% } \long\def\longpop@#1#2#3,#4\endargs@{% \long\def#1{#3}% \long\def#2{#4}% } %%%%%%%%%%%%%% End of code for > 10 arguments %%%%%%%%%%%%%%%%%% % This defines a Texinfo @macro or @rmacro, called by \parsemacbody. % \macrobody has the body of the macro in it, with placeholders for % its parameters, looking like "\xeatspaces{\hash 1}". % \paramno is the number of parameters % \paramlist is a TeX parameter text, e.g. "#1,#2,#3," % There are four cases: macros of zero, one, up to nine, and many arguments. % \xdef is used so that macro definitions will survive the file % they're defined in: @include reads the file inside a group. % \def\defmacro{% \let\hash=##% convert placeholders to macro parameter chars \ifnum\paramno=1 \def\xeatspaces##1{##1}% % This removes the pair of braces around the argument. We don't % use \eatspaces, because this can cause ends of lines to be lost % when the argument to \eatspaces is read, leading to line-based % commands like "@itemize" not being read correctly. \else \let\xeatspaces\relax % suppress expansion \fi \ifcase\paramno % 0 \expandafter\xdef\csname\the\macname\endcsname{% \noexpand\scanmacro{\macrobody}}% \or % 1 \expandafter\xdef\csname\the\macname\endcsname{% \bgroup \noexpand\braceorline \expandafter\noexpand\csname\the\macname @@@\endcsname}% \expandafter\xdef\csname\the\macname @@@\endcsname##1{% \egroup \noexpand\scanmacro{\macrobody}% }% \else % at most 9 \ifnum\paramno<10\relax % @MACNAME sets the context for reading the macro argument % @MACNAME@@ gets the argument, processes backslashes and appends a % comma. % @MACNAME@@@ removes braces surrounding the argument list. % @MACNAME@@@@ scans the macro body with arguments substituted. \expandafter\xdef\csname\the\macname\endcsname{% \bgroup \noexpand\expandafter % This \expandafter skip any spaces after the \noexpand\macroargctxt % macro before we change the catcode of space. \noexpand\expandafter \expandafter\noexpand\csname\the\macname @@\endcsname}% \expandafter\xdef\csname\the\macname @@\endcsname##1{% \noexpand\passargtomacro \expandafter\noexpand\csname\the\macname @@@\endcsname{##1,}}% \expandafter\xdef\csname\the\macname @@@\endcsname##1{% \expandafter\noexpand\csname\the\macname @@@@\endcsname ##1}% \expandafter\expandafter \expandafter\xdef \expandafter\expandafter \csname\the\macname @@@@\endcsname\paramlist{% \egroup\noexpand\scanmacro{\macrobody}}% \else % 10 or more: \expandafter\xdef\csname\the\macname\endcsname{% \noexpand\getargvals@{\the\macname}{\argl}% }% \global\expandafter\let\csname mac.\the\macname .body\endcsname\macrobody \global\expandafter\let\csname mac.\the\macname .recurse\endcsname\gobble \fi \fi} \catcode `\@\texiatcatcode\relax % end private-to-Texinfo catcodes \def\norecurse#1{\bgroup\cslet{#1}{macsave.#1}} %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % {\catcode`\@=0 \catcode`\\=13 % We need to manipulate \ so use @ as escape @catcode`@_=11 % private names @catcode`@!=11 % used as argument separator % \passargtomacro#1#2 - % Call #1 with a list of tokens #2, with any doubled backslashes in #2 % compressed to one. % % This implementation works by expansion, and not execution (so we cannot use % \def or similar). This reduces the risk of this failing in contexts where % complete expansion is done with no execution (for example, in writing out to % an auxiliary file for an index entry). % % State is kept in the input stream: the argument passed to % @look_ahead, @gobble_and_check_finish and @add_segment is % % THE_MACRO ARG_RESULT ! {PENDING_BS} NEXT_TOKEN (... rest of input) % % where: % THE_MACRO - name of the macro we want to call % ARG_RESULT - argument list we build to pass to that macro % PENDING_BS - either a backslash or nothing % NEXT_TOKEN - used to look ahead in the input stream to see what's coming next @gdef@passargtomacro#1#2{% @add_segment #1!{}@relax#2\@_finish\% } @gdef@_finish{@_finishx} @global@let@_finishx@relax % #1 - THE_MACRO ARG_RESULT % #2 - PENDING_BS % #3 - NEXT_TOKEN % #4 used to look ahead % % If the next token is not a backslash, process the rest of the argument; % otherwise, remove the next token. @gdef@look_ahead#1!#2#3#4{% @ifx#4\% @expandafter@gobble_and_check_finish @else @expandafter@add_segment @fi#1!{#2}#4#4% } % #1 - THE_MACRO ARG_RESULT % #2 - PENDING_BS % #3 - NEXT_TOKEN % #4 should be a backslash, which is gobbled. % #5 looks ahead % % Double backslash found. Add a single backslash, and look ahead. @gdef@gobble_and_check_finish#1!#2#3#4#5{% @add_segment#1\!{}#5#5% } @gdef@is_fi{@fi} % #1 - THE_MACRO ARG_RESULT % #2 - PENDING_BS % #3 - NEXT_TOKEN % #4 is input stream until next backslash % % Input stream is either at the start of the argument, or just after a % backslash sequence, either a lone backslash, or a doubled backslash. % NEXT_TOKEN contains the first token in the input stream: if it is \finish, % finish; otherwise, append to ARG_RESULT the segment of the argument up until % the next backslash. PENDING_BACKSLASH contains a backslash to represent % a backslash just before the start of the input stream that has not been % added to ARG_RESULT. @gdef@add_segment#1!#2#3#4\{% @ifx#3@_finish @call_the_macro#1!% @else % append the pending backslash to the result, followed by the next segment @expandafter@is_fi@look_ahead#1#2#4!{\}@fi % this @fi is discarded by @look_ahead. % we can't get rid of it with \expandafter because we don't know how % long #4 is. } % #1 - THE_MACRO % #2 - ARG_RESULT % #3 discards the res of the conditional in @add_segment, and @is_fi ends the % conditional. @gdef@call_the_macro#1#2!#3@fi{@is_fi #1{#2}} } %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % \braceorline MAC is used for a one-argument macro MAC. It checks % whether the next non-whitespace character is a {. It sets the context % for reading the argument (slightly different in the two cases). Then, % to read the argument, in the whole-line case, it then calls the regular % \parsearg MAC; in the lbrace case, it calls \passargtomacro MAC. % \def\braceorline#1{\let\macnamexxx=#1\futurelet\nchar\braceorlinexxx} \def\braceorlinexxx{% \ifx\nchar\bgroup \macroargctxt \expandafter\passargtomacro \else \macrolineargctxt\expandafter\parsearg \fi \macnamexxx} % @alias. % We need some trickery to remove the optional spaces around the equal % sign. Make them active and then expand them all to nothing. % \def\alias{\parseargusing\obeyspaces\aliasxxx} \def\aliasxxx #1{\aliasyyy#1\relax} \def\aliasyyy #1=#2\relax{% {% \expandafter\let\obeyedspace=\empty \addtomacrolist{#1}% \xdef\next{\global\let\makecsname{#1}=\makecsname{#2}}% }% \next } \message{cross references,} \newwrite\auxfile \newif\ifhavexrefs % True if xref values are known. \newif\ifwarnedxrefs % True if we warned once that they aren't known. % @inforef is relatively simple. \def\inforef #1{\inforefzzz #1,,,,**} \def\inforefzzz #1,#2,#3,#4**{% \putwordSee{} \putwordInfo{} \putwordfile{} \file{\ignorespaces #3{}}, node \samp{\ignorespaces#1{}}} % @node's only job in TeX is to define \lastnode, which is used in % cross-references. The @node line might or might not have commas, and % might or might not have spaces before the first comma, like: % @node foo , bar , ... % We don't want such trailing spaces in the node name. % \parseargdef\node{\checkenv{}\donode #1 ,\finishnodeparse} % % also remove a trailing comma, in case of something like this: % @node Help-Cross, , , Cross-refs \def\donode#1 ,#2\finishnodeparse{\dodonode #1,\finishnodeparse} \def\dodonode#1,#2\finishnodeparse{\gdef\lastnode{#1}} \let\nwnode=\node \let\lastnode=\empty % Write a cross-reference definition for the current node. #1 is the % type (Ynumbered, Yappendix, Ynothing). % \def\donoderef#1{% \ifx\lastnode\empty\else \setref{\lastnode}{#1}% \global\let\lastnode=\empty \fi } % @anchor{NAME} -- define xref target at arbitrary point. % \newcount\savesfregister % \def\savesf{\relax \ifhmode \savesfregister=\spacefactor \fi} \def\restoresf{\relax \ifhmode \spacefactor=\savesfregister \fi} \def\anchor#1{\savesf \setref{#1}{Ynothing}\restoresf \ignorespaces} % \setref{NAME}{SNT} defines a cross-reference point NAME (a node or an % anchor), which consists of three parts: % 1) NAME-title - the current sectioning name taken from \lastsection, % or the anchor name. % 2) NAME-snt - section number and type, passed as the SNT arg, or % empty for anchors. % 3) NAME-pg - the page number. % % This is called from \donoderef, \anchor, and \dofloat. In the case of % floats, there is an additional part, which is not written here: % 4) NAME-lof - the text as it should appear in a @listoffloats. % \def\setref#1#2{% \pdfmkdest{#1}% \iflinks {% \requireauxfile \atdummies % preserve commands, but don't expand them % match definition in \xrdef, \refx, \xrefX. \def\value##1{##1}% \edef\writexrdef##1##2{% \write\auxfile{@xrdef{#1-% #1 of \setref, expanded by the \edef ##1}{##2}}% these are parameters of \writexrdef }% \toks0 = \expandafter{\lastsection}% \immediate \writexrdef{title}{\the\toks0 }% \immediate \writexrdef{snt}{\csname #2\endcsname}% \Ynumbered etc. \safewhatsit{\writexrdef{pg}{\folio}}% will be written later, at \shipout }% \fi } % @xrefautosectiontitle on|off says whether @section(ing) names are used % automatically in xrefs, if the third arg is not explicitly specified. % This was provided as a "secret" @set xref-automatic-section-title % variable, now it's official. % \parseargdef\xrefautomaticsectiontitle{% \def\temp{#1}% \ifx\temp\onword \expandafter\let\csname SETxref-automatic-section-title\endcsname = \empty \else\ifx\temp\offword \expandafter\let\csname SETxref-automatic-section-title\endcsname = \relax \else \errhelp = \EMsimple \errmessage{Unknown @xrefautomaticsectiontitle value `\temp', must be on|off}% \fi\fi } % % @xref, @pxref, and @ref generate cross-references. For \xrefX, #1 is % the node name, #2 the name of the Info cross-reference, #3 the printed % node name, #4 the name of the Info file, #5 the name of the printed % manual. All but the node name can be omitted. % \def\pxref{\putwordsee{} \xrefXX} \def\xref{\putwordSee{} \xrefXX} \def\ref{\xrefXX} \def\xrefXX#1{\def\xrefXXarg{#1}\futurelet\tokenafterxref\xrefXXX} \def\xrefXXX{\expandafter\xrefX\expandafter[\xrefXXarg,,,,,,,]} % \newbox\toprefbox \newbox\printedrefnamebox \newbox\infofilenamebox \newbox\printedmanualbox % \def\xrefX[#1,#2,#3,#4,#5,#6]{\begingroup \unsepspaces % % Get args without leading/trailing spaces. \def\printedrefname{\ignorespaces #3}% \setbox\printedrefnamebox = \hbox{\printedrefname\unskip}% % \def\infofilename{\ignorespaces #4}% \setbox\infofilenamebox = \hbox{\infofilename\unskip}% % \def\printedmanual{\ignorespaces #5}% \setbox\printedmanualbox = \hbox{\printedmanual\unskip}% % % If the printed reference name (arg #3) was not explicitly given in % the @xref, figure out what we want to use. \ifdim \wd\printedrefnamebox = 0pt % No printed node name was explicitly given. \expandafter\ifx\csname SETxref-automatic-section-title\endcsname \relax % Not auto section-title: use node name inside the square brackets. \def\printedrefname{\ignorespaces #1}% \else % Auto section-title: use chapter/section title inside % the square brackets if we have it. \ifdim \wd\printedmanualbox > 0pt % It is in another manual, so we don't have it; use node name. \def\printedrefname{\ignorespaces #1}% \else \ifhavexrefs % We (should) know the real title if we have the xref values. \def\printedrefname{\refx{#1-title}{}}% \else % Otherwise just copy the Info node name. \def\printedrefname{\ignorespaces #1}% \fi% \fi \fi \fi % % Make link in pdf output. \ifpdf % For pdfTeX and LuaTeX {\indexnofonts \makevalueexpandable \turnoffactive % This expands tokens, so do it after making catcode changes, so _ % etc. don't get their TeX definitions. This ignores all spaces in % #4, including (wrongly) those in the middle of the filename. \getfilename{#4}% % % This (wrongly) does not take account of leading or trailing % spaces in #1, which should be ignored. \setpdfdestname{#1}% % \ifx\pdfdestname\empty \def\pdfdestname{Top}% no empty targets \fi % \leavevmode \startlink attr{/Border [0 0 0]}% \ifnum\filenamelength>0 goto file{\the\filename.pdf} name{\pdfdestname}% \else goto name{\pdfmkpgn{\pdfdestname}}% \fi }% \setcolor{\linkcolor}% \else \ifx\XeTeXrevision\thisisundefined \else % For XeTeX {\indexnofonts \makevalueexpandable \turnoffactive % This expands tokens, so do it after making catcode changes, so _ % etc. don't get their TeX definitions. This ignores all spaces in % #4, including (wrongly) those in the middle of the filename. \getfilename{#4}% % % This (wrongly) does not take account of leading or trailing % spaces in #1, which should be ignored. \setpdfdestname{#1}% % \ifx\pdfdestname\empty \def\pdfdestname{Top}% no empty targets \fi % \leavevmode \ifnum\filenamelength>0 % With default settings, % XeTeX (xdvipdfmx) replaces link destination names with integers. % In this case, the replaced destination names of % remote PDFs are no longer known. In order to avoid a replacement, % you can use xdvipdfmx's command line option `-C 0x0010'. % If you use XeTeX 0.99996+ (TeX Live 2016+), % this command line option is no longer necessary % because we can use the `dvipdfmx:config' special. \special{pdf:bann << /Border [0 0 0] /Type /Annot /Subtype /Link /A << /S /GoToR /F (\the\filename.pdf) /D (\pdfdestname) >> >>}% \else \special{pdf:bann << /Border [0 0 0] /Type /Annot /Subtype /Link /A << /S /GoTo /D (\pdfdestname) >> >>}% \fi }% \setcolor{\linkcolor}% \fi \fi {% % Have to otherify everything special to allow the \csname to % include an _ in the xref name, etc. \indexnofonts \turnoffactive \def\value##1{##1}% \expandafter\global\expandafter\let\expandafter\Xthisreftitle \csname XR#1-title\endcsname }% % % Float references are printed completely differently: "Figure 1.2" % instead of "[somenode], p.3". \iffloat distinguishes them by % \Xthisreftitle being set to a magic string. \iffloat\Xthisreftitle % If the user specified the print name (third arg) to the ref, % print it instead of our usual "Figure 1.2". \ifdim\wd\printedrefnamebox = 0pt \refx{#1-snt}{}% \else \printedrefname \fi % % If the user also gave the printed manual name (fifth arg), append % "in MANUALNAME". \ifdim \wd\printedmanualbox > 0pt \space \putwordin{} \cite{\printedmanual}% \fi \else % node/anchor (non-float) references. % % If we use \unhbox to print the node names, TeX does not insert % empty discretionaries after hyphens, which means that it will not % find a line break at a hyphen in a node names. Since some manuals % are best written with fairly long node names, containing hyphens, % this is a loss. Therefore, we give the text of the node name % again, so it is as if TeX is seeing it for the first time. % \ifdim \wd\printedmanualbox > 0pt % Cross-manual reference with a printed manual name. % \crossmanualxref{\cite{\printedmanual\unskip}}% % \else\ifdim \wd\infofilenamebox > 0pt % Cross-manual reference with only an info filename (arg 4), no % printed manual name (arg 5). This is essentially the same as % the case above; we output the filename, since we have nothing else. % \crossmanualxref{\code{\infofilename\unskip}}% % \else % Reference within this manual. % % _ (for example) has to be the character _ for the purposes of the % control sequence corresponding to the node, but it has to expand % into the usual \leavevmode...\vrule stuff for purposes of % printing. So we \turnoffactive for the \refx-snt, back on for the % printing, back off for the \refx-pg. {\turnoffactive % Only output a following space if the -snt ref is nonempty; for % @unnumbered and @anchor, it won't be. \setbox2 = \hbox{\ignorespaces \refx{#1-snt}{}}% \ifdim \wd2 > 0pt \refx{#1-snt}\space\fi }% % output the `[mynode]' via the macro below so it can be overridden. \xrefprintnodename\printedrefname % % But we always want a comma and a space: ,\space % % output the `page 3'. \turnoffactive \putwordpage\tie\refx{#1-pg}{}% % Add a , if xref followed by a space \if\space\noexpand\tokenafterxref ,% \else\ifx\ \tokenafterxref ,% @TAB \else\ifx\*\tokenafterxref ,% @* \else\ifx\ \tokenafterxref ,% @SPACE \else\ifx\ \tokenafterxref ,% @NL \else\ifx\tie\tokenafterxref ,% @tie \fi\fi\fi\fi\fi\fi \fi\fi \fi \endlink \endgroup} % Output a cross-manual xref to #1. Used just above (twice). % % Only include the text "Section ``foo'' in" if the foo is neither % missing or Top. Thus, @xref{,,,foo,The Foo Manual} outputs simply % "see The Foo Manual", the idea being to refer to the whole manual. % % But, this being TeX, we can't easily compare our node name against the % string "Top" while ignoring the possible spaces before and after in % the input. By adding the arbitrary 7sp below, we make it much less % likely that a real node name would have the same width as "Top" (e.g., % in a monospaced font). Hopefully it will never happen in practice. % % For the same basic reason, we retypeset the "Top" at every % reference, since the current font is indeterminate. % \def\crossmanualxref#1{% \setbox\toprefbox = \hbox{Top\kern7sp}% \setbox2 = \hbox{\ignorespaces \printedrefname \unskip \kern7sp}% \ifdim \wd2 > 7sp % nonempty? \ifdim \wd2 = \wd\toprefbox \else % same as Top? \putwordSection{} ``\printedrefname'' \putwordin{}\space \fi \fi #1% } % This macro is called from \xrefX for the `[nodename]' part of xref % output. It's a separate macro only so it can be changed more easily, % since square brackets don't work well in some documents. Particularly % one that Bob is working on :). % \def\xrefprintnodename#1{[#1]} % Things referred to by \setref. % \def\Ynothing{} \def\Yomitfromtoc{} \def\Ynumbered{% \ifnum\secno=0 \putwordChapter@tie \the\chapno \else \ifnum\subsecno=0 \putwordSection@tie \the\chapno.\the\secno \else \ifnum\subsubsecno=0 \putwordSection@tie \the\chapno.\the\secno.\the\subsecno \else \putwordSection@tie \the\chapno.\the\secno.\the\subsecno.\the\subsubsecno \fi\fi\fi } \def\Yappendix{% \ifnum\secno=0 \putwordAppendix@tie @char\the\appendixno{}% \else \ifnum\subsecno=0 \putwordSection@tie @char\the\appendixno.\the\secno \else \ifnum\subsubsecno=0 \putwordSection@tie @char\the\appendixno.\the\secno.\the\subsecno \else \putwordSection@tie @char\the\appendixno.\the\secno.\the\subsecno.\the\subsubsecno \fi\fi\fi } % \refx{NAME}{SUFFIX} - reference a cross-reference string named NAME. SUFFIX % is output afterwards if non-empty. \def\refx#1#2{% \requireauxfile {% \indexnofonts \otherbackslash \def\value##1{##1}% \expandafter\global\expandafter\let\expandafter\thisrefX \csname XR#1\endcsname }% \ifx\thisrefX\relax % If not defined, say something at least. \angleleft un\-de\-fined\angleright \iflinks \ifhavexrefs {\toks0 = {#1}% avoid expansion of possibly-complex value \message{\linenumber Undefined cross reference `\the\toks0'.}}% \else \ifwarnedxrefs\else \global\warnedxrefstrue \message{Cross reference values unknown; you must run TeX again.}% \fi \fi \fi \else % It's defined, so just use it. \thisrefX \fi #2% Output the suffix in any case. } % This is the macro invoked by entries in the aux file. Define a control % sequence for a cross-reference target (we prepend XR to the control sequence % name to avoid collisions). The value is the page number. If this is a float % type, we have more work to do. % \def\xrdef#1#2{% {% Expand the node or anchor name to remove control sequences. % \turnoffactive stops 8-bit characters being changed to commands % like @'e. \refx does the same to retrieve the value in the definition. \indexnofonts \turnoffactive \def\value##1{##1}% \xdef\safexrefname{#1}% }% % \expandafter\gdef\csname XR\safexrefname\endcsname{#2}% remember this xref % % Was that xref control sequence that we just defined for a float? \expandafter\iffloat\csname XR\safexrefname\endcsname % it was a float, and we have the (safe) float type in \iffloattype. \expandafter\let\expandafter\floatlist \csname floatlist\iffloattype\endcsname % % Is this the first time we've seen this float type? \expandafter\ifx\floatlist\relax \toks0 = {\do}% yes, so just \do \else % had it before, so preserve previous elements in list. \toks0 = \expandafter{\floatlist\do}% \fi % % Remember this xref in the control sequence \floatlistFLOATTYPE, % for later use in \listoffloats. \expandafter\xdef\csname floatlist\iffloattype\endcsname{\the\toks0 {\safexrefname}}% \fi } % If working on a large document in chapters, it is convenient to % be able to disable indexing, cross-referencing, and contents, for test runs. % This is done with @novalidate at the beginning of the file. % \newif\iflinks \linkstrue % by default we want the aux files. \let\novalidate = \linksfalse % Used when writing to the aux file, or when using data from it. \def\requireauxfile{% \iflinks \tryauxfile % Open the new aux file. TeX will close it automatically at exit. \immediate\openout\auxfile=\jobname.aux \fi \global\let\requireauxfile=\relax % Only do this once. } % Read the last existing aux file, if any. No error if none exists. % \def\tryauxfile{% \openin 1 \jobname.aux \ifeof 1 \else \readdatafile{aux}% \global\havexrefstrue \fi \closein 1 } \def\setupdatafile{% \catcode`\^^@=\other \catcode`\^^A=\other \catcode`\^^B=\other \catcode`\^^C=\other \catcode`\^^D=\other \catcode`\^^E=\other \catcode`\^^F=\other \catcode`\^^G=\other \catcode`\^^H=\other \catcode`\^^K=\other \catcode`\^^L=\other \catcode`\^^N=\other \catcode`\^^P=\other \catcode`\^^Q=\other \catcode`\^^R=\other \catcode`\^^S=\other \catcode`\^^T=\other \catcode`\^^U=\other \catcode`\^^V=\other \catcode`\^^W=\other \catcode`\^^X=\other \catcode`\^^Z=\other \catcode`\^^[=\other \catcode`\^^\=\other \catcode`\^^]=\other \catcode`\^^^=\other \catcode`\^^_=\other % It was suggested to set the catcode of ^ to 7, which would allow ^^e4 etc. % in xref tags, i.e., node names. But since ^^e4 notation isn't % supported in the main text, it doesn't seem desirable. Furthermore, % that is not enough: for node names that actually contain a ^ % character, we would end up writing a line like this: 'xrdef {'hat % b-title}{'hat b} and \xrdef does a \csname...\endcsname on the first % argument, and \hat is not an expandable control sequence. It could % all be worked out, but why? Either we support ^^ or we don't. % % The other change necessary for this was to define \auxhat: % \def\auxhat{\def^{'hat }}% extra space so ok if followed by letter % and then to call \auxhat in \setq. % \catcode`\^=\other % % Special characters. Should be turned off anyway, but... \catcode`\~=\other \catcode`\[=\other \catcode`\]=\other \catcode`\"=\other \catcode`\_=\other \catcode`\|=\other \catcode`\<=\other \catcode`\>=\other \catcode`\$=\other \catcode`\#=\other \catcode`\&=\other \catcode`\%=\other \catcode`+=\other % avoid \+ for paranoia even though we've turned it off % % This is to support \ in node names and titles, since the \ % characters end up in a \csname. It's easier than % leaving it active and making its active definition an actual \ % character. What I don't understand is why it works in the *value* % of the xrdef. Seems like it should be a catcode12 \, and that % should not typeset properly. But it works, so I'm moving on for % now. --karl, 15jan04. \catcode`\\=\other % % @ is our escape character in .aux files, and we need braces. \catcode`\{=1 \catcode`\}=2 \catcode`\@=0 } \def\readdatafile#1{% \begingroup \setupdatafile \input\jobname.#1 \endgroup} \message{insertions,} % including footnotes. \newcount \footnoteno % The trailing space in the following definition for supereject is % vital for proper filling; pages come out unaligned when you do a % pagealignmacro call if that space before the closing brace is % removed. (Generally, numeric constants should always be followed by a % space to prevent strange expansion errors.) \def\supereject{\par\penalty -20000\footnoteno =0 } % @footnotestyle is meaningful for Info output only. \let\footnotestyle=\comment {\catcode `\@=11 % % Auto-number footnotes. Otherwise like plain. \gdef\footnote{% \global\advance\footnoteno by \@ne \edef\thisfootno{$^{\the\footnoteno}$}% % % In case the footnote comes at the end of a sentence, preserve the % extra spacing after we do the footnote number. \let\@sf\empty \ifhmode\edef\@sf{\spacefactor\the\spacefactor}\ptexslash\fi % % Remove inadvertent blank space before typesetting the footnote number. \unskip \thisfootno\@sf \dofootnote }% % Don't bother with the trickery in plain.tex to not require the % footnote text as a parameter. Our footnotes don't need to be so general. % % Oh yes, they do; otherwise, @ifset (and anything else that uses % \parseargline) fails inside footnotes because the tokens are fixed when % the footnote is read. --karl, 16nov96. % \gdef\dofootnote{% \insert\footins\bgroup % % Nested footnotes are not supported in TeX, that would take a lot % more work. (\startsavinginserts does not suffice.) \let\footnote=\errfootnotenest % % We want to typeset this text as a normal paragraph, even if the % footnote reference occurs in (for example) a display environment. % So reset some parameters. \hsize=\txipagewidth \interlinepenalty\interfootnotelinepenalty \splittopskip\ht\strutbox % top baseline for broken footnotes \splitmaxdepth\dp\strutbox \floatingpenalty\@MM \leftskip\z@skip \rightskip\z@skip \spaceskip\z@skip \xspaceskip\z@skip \parindent\defaultparindent % \smallfonts \rm % % Because we use hanging indentation in footnotes, a @noindent appears % to exdent this text, so make it be a no-op. makeinfo does not use % hanging indentation so @noindent can still be needed within footnote % text after an @example or the like (not that this is good style). \let\noindent = \relax % % Hang the footnote text off the number. Use \everypar in case the % footnote extends for more than one paragraph. \everypar = {\hang}% \textindent{\thisfootno}% % % Don't crash into the line above the footnote text. Since this % expands into a box, it must come within the paragraph, lest it % provide a place where TeX can split the footnote. \footstrut % % Invoke rest of plain TeX footnote routine. \futurelet\next\fo@t } }%end \catcode `\@=11 \def\errfootnotenest{% \errhelp=\EMsimple \errmessage{Nested footnotes not supported in texinfo.tex, even though they work in makeinfo; sorry} } \def\errfootnoteheading{% \errhelp=\EMsimple \errmessage{Footnotes in chapters, sections, etc., are not supported} } % In case a @footnote appears in a vbox, save the footnote text and create % the real \insert just after the vbox finished. Otherwise, the insertion % would be lost. % Similarly, if a @footnote appears inside an alignment, save the footnote % text to a box and make the \insert when a row of the table is finished. % And the same can be done for other insert classes. --kasal, 16nov03. % % Replace the \insert primitive by a cheating macro. % Deeper inside, just make sure that the saved insertions are not spilled % out prematurely. % \def\startsavinginserts{% \ifx \insert\ptexinsert \let\insert\saveinsert \else \let\checkinserts\relax \fi } % This \insert replacement works for both \insert\footins{foo} and % \insert\footins\bgroup foo\egroup, but it doesn't work for \insert27{foo}. % \def\saveinsert#1{% \edef\next{\noexpand\savetobox \makeSAVEname#1}% \afterassignment\next % swallow the left brace \let\temp = } \def\makeSAVEname#1{\makecsname{SAVE\expandafter\gobble\string#1}} \def\savetobox#1{\global\setbox#1 = \vbox\bgroup \unvbox#1} \def\checksaveins#1{\ifvoid#1\else \placesaveins#1\fi} \def\placesaveins#1{% \ptexinsert \csname\expandafter\gobblesave\string#1\endcsname {\box#1}% } % eat @SAVE -- beware, all of them have catcode \other: { \def\dospecials{\do S\do A\do V\do E} \uncatcodespecials % ;-) \gdef\gobblesave @SAVE{} } % initialization: \def\newsaveins #1{% \edef\next{\noexpand\newsaveinsX \makeSAVEname#1}% \next } \def\newsaveinsX #1{% \csname newbox\endcsname #1% \expandafter\def\expandafter\checkinserts\expandafter{\checkinserts \checksaveins #1}% } % initialize: \let\checkinserts\empty \newsaveins\footins \newsaveins\margin % @image. We use the macros from epsf.tex to support this. % If epsf.tex is not installed and @image is used, we complain. % % Check for and read epsf.tex up front. If we read it only at @image % time, we might be inside a group, and then its definitions would get % undone and the next image would fail. \openin 1 = epsf.tex \ifeof 1 \else % Do not bother showing banner with epsf.tex v2.7k (available in % doc/epsf.tex and on ctan). \def\epsfannounce{\toks0 = }% \input epsf.tex \fi \closein 1 % % We will only complain once about lack of epsf.tex. \newif\ifwarnednoepsf \newhelp\noepsfhelp{epsf.tex must be installed for images to work. It is also included in the Texinfo distribution, or you can get it from ftp://tug.org/tex/epsf.tex.} % \def\image#1{% \ifx\epsfbox\thisisundefined \ifwarnednoepsf \else \errhelp = \noepsfhelp \errmessage{epsf.tex not found, images will be ignored}% \global\warnednoepsftrue \fi \else \imagexxx #1,,,,,\finish \fi } % % Arguments to @image: % #1 is (mandatory) image filename; we tack on .eps extension. % #2 is (optional) width, #3 is (optional) height. % #4 is (ignored optional) html alt text. % #5 is (ignored optional) extension. % #6 is just the usual extra ignored arg for parsing stuff. \newif\ifimagevmode \def\imagexxx#1,#2,#3,#4,#5,#6\finish{\begingroup \catcode`\^^M = 5 % in case we're inside an example \normalturnoffactive % allow _ et al. in names \def\xprocessmacroarg{\eatspaces}% in case we are being used via a macro % If the image is by itself, center it. \ifvmode \imagevmodetrue \else \ifx\centersub\centerV % for @center @image, we need a vbox so we can have our vertical space \imagevmodetrue \vbox\bgroup % vbox has better behavior than vtop herev \fi\fi % \ifimagevmode \nobreak\medskip % Usually we'll have text after the image which will insert % \parskip glue, so insert it here too to equalize the space % above and below. \nobreak\vskip\parskip \nobreak \fi % % Leave vertical mode so that indentation from an enclosing % environment such as @quotation is respected. % However, if we're at the top level, we don't want the % normal paragraph indentation. % On the other hand, if we are in the case of @center @image, we don't % want to start a paragraph, which will create a hsize-width box and % eradicate the centering. \ifx\centersub\centerV\else \noindent \fi % % Output the image. \ifpdf % For pdfTeX and LuaTeX <= 0.80 \dopdfimage{#1}{#2}{#3}% \else \ifx\XeTeXrevision\thisisundefined % For epsf.tex % \epsfbox itself resets \epsf?size at each figure. \setbox0 = \hbox{\ignorespaces #2}% \ifdim\wd0 > 0pt \epsfxsize=#2\relax \fi \setbox0 = \hbox{\ignorespaces #3}% \ifdim\wd0 > 0pt \epsfysize=#3\relax \fi \epsfbox{#1.eps}% \else % For XeTeX \doxeteximage{#1}{#2}{#3}% \fi \fi % \ifimagevmode \medskip % space after a standalone image \fi \ifx\centersub\centerV \egroup \fi \endgroup} % @float FLOATTYPE,LABEL,LOC ... @end float for displayed figures, tables, % etc. We don't actually implement floating yet, we always include the % float "here". But it seemed the best name for the future. % \envparseargdef\float{\eatcommaspace\eatcommaspace\dofloat#1, , ,\finish} % There may be a space before second and/or third parameter; delete it. \def\eatcommaspace#1, {#1,} % #1 is the optional FLOATTYPE, the text label for this float, typically % "Figure", "Table", "Example", etc. Can't contain commas. If omitted, % this float will not be numbered and cannot be referred to. % % #2 is the optional xref label. Also must be present for the float to % be referable. % % #3 is the optional positioning argument; for now, it is ignored. It % will somehow specify the positions allowed to float to (here, top, bottom). % % We keep a separate counter for each FLOATTYPE, which we reset at each % chapter-level command. \let\resetallfloatnos=\empty % \def\dofloat#1,#2,#3,#4\finish{% \let\thiscaption=\empty \let\thisshortcaption=\empty % % don't lose footnotes inside @float. % % BEWARE: when the floats start float, we have to issue warning whenever an % insert appears inside a float which could possibly float. --kasal, 26may04 % \startsavinginserts % % We can't be used inside a paragraph. \par % \vtop\bgroup \def\floattype{#1}% \def\floatlabel{#2}% \def\floatloc{#3}% we do nothing with this yet. % \ifx\floattype\empty \let\safefloattype=\empty \else {% % the floattype might have accents or other special characters, % but we need to use it in a control sequence name. \indexnofonts \turnoffactive \xdef\safefloattype{\floattype}% }% \fi % % If label is given but no type, we handle that as the empty type. \ifx\floatlabel\empty \else % We want each FLOATTYPE to be numbered separately (Figure 1, % Table 1, Figure 2, ...). (And if no label, no number.) % \expandafter\getfloatno\csname\safefloattype floatno\endcsname \global\advance\floatno by 1 % {% % This magic value for \lastsection is output by \setref as the % XREFLABEL-title value. \xrefX uses it to distinguish float % labels (which have a completely different output format) from % node and anchor labels. And \xrdef uses it to construct the % lists of floats. % \edef\lastsection{\floatmagic=\safefloattype}% \setref{\floatlabel}{Yfloat}% }% \fi % % start with \parskip glue, I guess. \vskip\parskip % % Don't suppress indentation if a float happens to start a section. \restorefirstparagraphindent } % we have these possibilities: % @float Foo,lbl & @caption{Cap}: Foo 1.1: Cap % @float Foo,lbl & no caption: Foo 1.1 % @float Foo & @caption{Cap}: Foo: Cap % @float Foo & no caption: Foo % @float ,lbl & Caption{Cap}: 1.1: Cap % @float ,lbl & no caption: 1.1 % @float & @caption{Cap}: Cap % @float & no caption: % \def\Efloat{% \let\floatident = \empty % % In all cases, if we have a float type, it comes first. \ifx\floattype\empty \else \def\floatident{\floattype}\fi % % If we have an xref label, the number comes next. \ifx\floatlabel\empty \else \ifx\floattype\empty \else % if also had float type, need tie first. \appendtomacro\floatident{\tie}% \fi % the number. \appendtomacro\floatident{\chaplevelprefix\the\floatno}% \fi % % Start the printed caption with what we've constructed in % \floatident, but keep it separate; we need \floatident again. \let\captionline = \floatident % \ifx\thiscaption\empty \else \ifx\floatident\empty \else \appendtomacro\captionline{: }% had ident, so need a colon between \fi % % caption text. \appendtomacro\captionline{\scanexp\thiscaption}% \fi % % If we have anything to print, print it, with space before. % Eventually this needs to become an \insert. \ifx\captionline\empty \else \vskip.5\parskip \captionline % % Space below caption. \vskip\parskip \fi % % If have an xref label, write the list of floats info. Do this % after the caption, to avoid chance of it being a breakpoint. \ifx\floatlabel\empty \else % Write the text that goes in the lof to the aux file as % \floatlabel-lof. Besides \floatident, we include the short % caption if specified, else the full caption if specified, else nothing. {% \requireauxfile \atdummies % \ifx\thisshortcaption\empty \def\gtemp{\thiscaption}% \else \def\gtemp{\thisshortcaption}% \fi \immediate\write\auxfile{@xrdef{\floatlabel-lof}{\floatident \ifx\gtemp\empty \else : \gtemp \fi}}% }% \fi \egroup % end of \vtop % \checkinserts } % Append the tokens #2 to the definition of macro #1, not expanding either. % \def\appendtomacro#1#2{% \expandafter\def\expandafter#1\expandafter{#1#2}% } % @caption, @shortcaption % \def\caption{\docaption\thiscaption} \def\shortcaption{\docaption\thisshortcaption} \def\docaption{\checkenv\float \bgroup\scanargctxt\defcaption} \def\defcaption#1#2{\egroup \def#1{#2}} % The parameter is the control sequence identifying the counter we are % going to use. Create it if it doesn't exist and assign it to \floatno. \def\getfloatno#1{% \ifx#1\relax % Haven't seen this figure type before. \csname newcount\endcsname #1% % % Remember to reset this floatno at the next chap. \expandafter\gdef\expandafter\resetallfloatnos \expandafter{\resetallfloatnos #1=0 }% \fi \let\floatno#1% } % \setref calls this to get the XREFLABEL-snt value. We want an @xref % to the FLOATLABEL to expand to "Figure 3.1". We call \setref when we % first read the @float command. % \def\Yfloat{\floattype@tie \chaplevelprefix\the\floatno}% % Magic string used for the XREFLABEL-title value, so \xrefX can % distinguish floats from other xref types. \def\floatmagic{!!float!!} % #1 is the control sequence we are passed; we expand into a conditional % which is true if #1 represents a float ref. That is, the magic % \lastsection value which we \setref above. % \def\iffloat#1{\expandafter\doiffloat#1==\finish} % % #1 is (maybe) the \floatmagic string. If so, #2 will be the % (safe) float type for this float. We set \iffloattype to #2. % \def\doiffloat#1=#2=#3\finish{% \def\temp{#1}% \def\iffloattype{#2}% \ifx\temp\floatmagic } % @listoffloats FLOATTYPE - print a list of floats like a table of contents. % \parseargdef\listoffloats{% \def\floattype{#1}% floattype {% % the floattype might have accents or other special characters, % but we need to use it in a control sequence name. \indexnofonts \turnoffactive \xdef\safefloattype{\floattype}% }% % % \xrdef saves the floats as a \do-list in \floatlistSAFEFLOATTYPE. \expandafter\ifx\csname floatlist\safefloattype\endcsname \relax \ifhavexrefs % if the user said @listoffloats foo but never @float foo. \message{\linenumber No `\safefloattype' floats to list.}% \fi \else \begingroup \leftskip=\tocindent % indent these entries like a toc \let\do=\listoffloatsdo \csname floatlist\safefloattype\endcsname \endgroup \fi } % This is called on each entry in a list of floats. We're passed the % xref label, in the form LABEL-title, which is how we save it in the % aux file. We strip off the -title and look up \XRLABEL-lof, which % has the text we're supposed to typeset here. % % Figures without xref labels will not be included in the list (since % they won't appear in the aux file). % \def\listoffloatsdo#1{\listoffloatsdoentry#1\finish} \def\listoffloatsdoentry#1-title\finish{{% % Can't fully expand XR#1-lof because it can contain anything. Just % pass the control sequence. On the other hand, XR#1-pg is just the % page number, and we want to fully expand that so we can get a link % in pdf output. \toksA = \expandafter{\csname XR#1-lof\endcsname}% % % use the same \entry macro we use to generate the TOC and index. \edef\writeentry{\noexpand\entry{\the\toksA}{\csname XR#1-pg\endcsname}}% \writeentry }} \message{localization,} % For single-language documents, @documentlanguage is usually given very % early, just after @documentencoding. Single argument is the language % (de) or locale (de_DE) abbreviation. % { \catcode`\_ = \active \globaldefs=1 \parseargdef\documentlanguage{% \tex % read txi-??.tex file in plain TeX. % Read the file by the name they passed if it exists. \let_ = \normalunderscore % normal _ character for filename test \openin 1 txi-#1.tex \ifeof 1 \documentlanguagetrywithoutunderscore #1_\finish \else \globaldefs = 1 % everything in the txi-LL files needs to persist \input txi-#1.tex \fi \closein 1 \endgroup % end raw TeX } % % If they passed de_DE, and txi-de_DE.tex doesn't exist, % try txi-de.tex. % \gdef\documentlanguagetrywithoutunderscore#1_#2\finish{% \openin 1 txi-#1.tex \ifeof 1 \errhelp = \nolanghelp \errmessage{Cannot read language file txi-#1.tex}% \else \globaldefs = 1 % everything in the txi-LL files needs to persist \input txi-#1.tex \fi \closein 1 } }% end of special _ catcode % \newhelp\nolanghelp{The given language definition file cannot be found or is empty. Maybe you need to install it? Putting it in the current directory should work if nowhere else does.} % This macro is called from txi-??.tex files; the first argument is the % \language name to set (without the "\lang@" prefix), the second and % third args are \{left,right}hyphenmin. % % The language names to pass are determined when the format is built. % See the etex.log file created at that time, e.g., % /usr/local/texlive/2008/texmf-var/web2c/pdftex/etex.log. % % With TeX Live 2008, etex now includes hyphenation patterns for all % available languages. This means we can support hyphenation in % Texinfo, at least to some extent. (This still doesn't solve the % accented characters problem.) % \catcode`@=11 \def\txisetlanguage#1#2#3{% % do not set the language if the name is undefined in the current TeX. \expandafter\ifx\csname lang@#1\endcsname \relax \message{no patterns for #1}% \else \global\language = \csname lang@#1\endcsname \fi % but there is no harm in adjusting the hyphenmin values regardless. \global\lefthyphenmin = #2\relax \global\righthyphenmin = #3\relax } % XeTeX and LuaTeX can handle Unicode natively. % Their default I/O uses UTF-8 sequences instead of a byte-wise operation. % Other TeX engines' I/O (pdfTeX, etc.) is byte-wise. % \newif\iftxinativeunicodecapable \newif\iftxiusebytewiseio \ifx\XeTeXrevision\thisisundefined \ifx\luatexversion\thisisundefined \txinativeunicodecapablefalse \txiusebytewiseiotrue \else \txinativeunicodecapabletrue \txiusebytewiseiofalse \fi \else \txinativeunicodecapabletrue \txiusebytewiseiofalse \fi % Set I/O by bytes instead of UTF-8 sequence for XeTeX and LuaTex % for non-UTF-8 (byte-wise) encodings. % \def\setbytewiseio{% \ifx\XeTeXrevision\thisisundefined \else \XeTeXdefaultencoding "bytes" % For subsequent files to be read \XeTeXinputencoding "bytes" % For document root file % Unfortunately, there seems to be no corresponding XeTeX command for % output encoding. This is a problem for auxiliary index and TOC files. % The only solution would be perhaps to write out @U{...} sequences in % place of non-ASCII characters. \fi \ifx\luatexversion\thisisundefined \else \directlua{ local utf8_char, byte, gsub = unicode.utf8.char, string.byte, string.gsub local function convert_char (char) return utf8_char(byte(char)) end local function convert_line (line) return gsub(line, ".", convert_char) end callback.register("process_input_buffer", convert_line) local function convert_line_out (line) local line_out = "" for c in string.utfvalues(line) do line_out = line_out .. string.char(c) end return line_out end callback.register("process_output_buffer", convert_line_out) } \fi \txiusebytewiseiotrue } % Helpers for encodings. % Set the catcode of characters 128 through 255 to the specified number. % \def\setnonasciicharscatcode#1{% \count255=128 \loop\ifnum\count255<256 \global\catcode\count255=#1\relax \advance\count255 by 1 \repeat } \def\setnonasciicharscatcodenonglobal#1{% \count255=128 \loop\ifnum\count255<256 \catcode\count255=#1\relax \advance\count255 by 1 \repeat } % @documentencoding sets the definition of non-ASCII characters % according to the specified encoding. % \def\documentencoding{\parseargusing\filenamecatcodes\documentencodingzzz} \def\documentencodingzzz#1{% % % Encoding being declared for the document. \def\declaredencoding{\csname #1.enc\endcsname}% % % Supported encodings: names converted to tokens in order to be able % to compare them with \ifx. \def\ascii{\csname US-ASCII.enc\endcsname}% \def\latnine{\csname ISO-8859-15.enc\endcsname}% \def\latone{\csname ISO-8859-1.enc\endcsname}% \def\lattwo{\csname ISO-8859-2.enc\endcsname}% \def\utfeight{\csname UTF-8.enc\endcsname}% % \ifx \declaredencoding \ascii \asciichardefs % \else \ifx \declaredencoding \lattwo \iftxinativeunicodecapable \setbytewiseio \fi \setnonasciicharscatcode\active \lattwochardefs % \else \ifx \declaredencoding \latone \iftxinativeunicodecapable \setbytewiseio \fi \setnonasciicharscatcode\active \latonechardefs % \else \ifx \declaredencoding \latnine \iftxinativeunicodecapable \setbytewiseio \fi \setnonasciicharscatcode\active \latninechardefs % \else \ifx \declaredencoding \utfeight \iftxinativeunicodecapable % For native Unicode handling (XeTeX and LuaTeX) \nativeunicodechardefs \else % For treating UTF-8 as byte sequences (TeX, eTeX and pdfTeX) \setnonasciicharscatcode\active % since we already invoked \utfeightchardefs at the top level % (below), do not re-invoke it, otherwise our check for duplicated % definitions gets triggered. Making non-ascii chars active is % sufficient. \fi % \else \message{Ignoring unknown document encoding: #1.}% % \fi % utfeight \fi % latnine \fi % latone \fi % lattwo \fi % ascii % \ifx\XeTeXrevision\thisisundefined \else \ifx \declaredencoding \utfeight \else \ifx \declaredencoding \ascii \else \message{Warning: XeTeX with non-UTF-8 encodings cannot handle % non-ASCII characters in auxiliary files.}% \fi \fi \fi } % emacs-page % A message to be logged when using a character that isn't available % the default font encoding (OT1). % \def\missingcharmsg#1{\message{Character missing, sorry: #1.}} % Take account of \c (plain) vs. \, (Texinfo) difference. \def\cedilla#1{\ifx\c\ptexc\c{#1}\else\,{#1}\fi} % First, make active non-ASCII characters in order for them to be % correctly categorized when TeX reads the replacement text of % macros containing the character definitions. \setnonasciicharscatcode\active % \def\gdefchar#1#2{% \gdef#1{% \ifpassthroughchars \string#1% \else #2% \fi }} % Latin1 (ISO-8859-1) character definitions. \def\latonechardefs{% \gdefchar^^a0{\tie} \gdefchar^^a1{\exclamdown} \gdefchar^^a2{{\tcfont \char162}} % cent \gdefchar^^a3{\pounds{}} \gdefchar^^a4{{\tcfont \char164}} % currency \gdefchar^^a5{{\tcfont \char165}} % yen \gdefchar^^a6{{\tcfont \char166}} % broken bar \gdefchar^^a7{\S} \gdefchar^^a8{\"{}} \gdefchar^^a9{\copyright{}} \gdefchar^^aa{\ordf} \gdefchar^^ab{\guillemetleft{}} \gdefchar^^ac{\ensuremath\lnot} \gdefchar^^ad{\-} \gdefchar^^ae{\registeredsymbol{}} \gdefchar^^af{\={}} % \gdefchar^^b0{\textdegree} \gdefchar^^b1{$\pm$} \gdefchar^^b2{$^2$} \gdefchar^^b3{$^3$} \gdefchar^^b4{\'{}} \gdefchar^^b5{$\mu$} \gdefchar^^b6{\P} \gdefchar^^b7{\ensuremath\cdot} \gdefchar^^b8{\cedilla\ } \gdefchar^^b9{$^1$} \gdefchar^^ba{\ordm} \gdefchar^^bb{\guillemetright{}} \gdefchar^^bc{$1\over4$} \gdefchar^^bd{$1\over2$} \gdefchar^^be{$3\over4$} \gdefchar^^bf{\questiondown} % \gdefchar^^c0{\`A} \gdefchar^^c1{\'A} \gdefchar^^c2{\^A} \gdefchar^^c3{\~A} \gdefchar^^c4{\"A} \gdefchar^^c5{\ringaccent A} \gdefchar^^c6{\AE} \gdefchar^^c7{\cedilla C} \gdefchar^^c8{\`E} \gdefchar^^c9{\'E} \gdefchar^^ca{\^E} \gdefchar^^cb{\"E} \gdefchar^^cc{\`I} \gdefchar^^cd{\'I} \gdefchar^^ce{\^I} \gdefchar^^cf{\"I} % \gdefchar^^d0{\DH} \gdefchar^^d1{\~N} \gdefchar^^d2{\`O} \gdefchar^^d3{\'O} \gdefchar^^d4{\^O} \gdefchar^^d5{\~O} \gdefchar^^d6{\"O} \gdefchar^^d7{$\times$} \gdefchar^^d8{\O} \gdefchar^^d9{\`U} \gdefchar^^da{\'U} \gdefchar^^db{\^U} \gdefchar^^dc{\"U} \gdefchar^^dd{\'Y} \gdefchar^^de{\TH} \gdefchar^^df{\ss} % \gdefchar^^e0{\`a} \gdefchar^^e1{\'a} \gdefchar^^e2{\^a} \gdefchar^^e3{\~a} \gdefchar^^e4{\"a} \gdefchar^^e5{\ringaccent a} \gdefchar^^e6{\ae} \gdefchar^^e7{\cedilla c} \gdefchar^^e8{\`e} \gdefchar^^e9{\'e} \gdefchar^^ea{\^e} \gdefchar^^eb{\"e} \gdefchar^^ec{\`{\dotless i}} \gdefchar^^ed{\'{\dotless i}} \gdefchar^^ee{\^{\dotless i}} \gdefchar^^ef{\"{\dotless i}} % \gdefchar^^f0{\dh} \gdefchar^^f1{\~n} \gdefchar^^f2{\`o} \gdefchar^^f3{\'o} \gdefchar^^f4{\^o} \gdefchar^^f5{\~o} \gdefchar^^f6{\"o} \gdefchar^^f7{$\div$} \gdefchar^^f8{\o} \gdefchar^^f9{\`u} \gdefchar^^fa{\'u} \gdefchar^^fb{\^u} \gdefchar^^fc{\"u} \gdefchar^^fd{\'y} \gdefchar^^fe{\th} \gdefchar^^ff{\"y} } % Latin9 (ISO-8859-15) encoding character definitions. \def\latninechardefs{% % Encoding is almost identical to Latin1. \latonechardefs % \gdefchar^^a4{\euro{}} \gdefchar^^a6{\v S} \gdefchar^^a8{\v s} \gdefchar^^b4{\v Z} \gdefchar^^b8{\v z} \gdefchar^^bc{\OE} \gdefchar^^bd{\oe} \gdefchar^^be{\"Y} } % Latin2 (ISO-8859-2) character definitions. \def\lattwochardefs{% \gdefchar^^a0{\tie} \gdefchar^^a1{\ogonek{A}} \gdefchar^^a2{\u{}} \gdefchar^^a3{\L} \gdefchar^^a4{\missingcharmsg{CURRENCY SIGN}} \gdefchar^^a5{\v L} \gdefchar^^a6{\'S} \gdefchar^^a7{\S} \gdefchar^^a8{\"{}} \gdefchar^^a9{\v S} \gdefchar^^aa{\cedilla S} \gdefchar^^ab{\v T} \gdefchar^^ac{\'Z} \gdefchar^^ad{\-} \gdefchar^^ae{\v Z} \gdefchar^^af{\dotaccent Z} % \gdefchar^^b0{\textdegree{}} \gdefchar^^b1{\ogonek{a}} \gdefchar^^b2{\ogonek{ }} \gdefchar^^b3{\l} \gdefchar^^b4{\'{}} \gdefchar^^b5{\v l} \gdefchar^^b6{\'s} \gdefchar^^b7{\v{}} \gdefchar^^b8{\cedilla\ } \gdefchar^^b9{\v s} \gdefchar^^ba{\cedilla s} \gdefchar^^bb{\v t} \gdefchar^^bc{\'z} \gdefchar^^bd{\H{}} \gdefchar^^be{\v z} \gdefchar^^bf{\dotaccent z} % \gdefchar^^c0{\'R} \gdefchar^^c1{\'A} \gdefchar^^c2{\^A} \gdefchar^^c3{\u A} \gdefchar^^c4{\"A} \gdefchar^^c5{\'L} \gdefchar^^c6{\'C} \gdefchar^^c7{\cedilla C} \gdefchar^^c8{\v C} \gdefchar^^c9{\'E} \gdefchar^^ca{\ogonek{E}} \gdefchar^^cb{\"E} \gdefchar^^cc{\v E} \gdefchar^^cd{\'I} \gdefchar^^ce{\^I} \gdefchar^^cf{\v D} % \gdefchar^^d0{\DH} \gdefchar^^d1{\'N} \gdefchar^^d2{\v N} \gdefchar^^d3{\'O} \gdefchar^^d4{\^O} \gdefchar^^d5{\H O} \gdefchar^^d6{\"O} \gdefchar^^d7{$\times$} \gdefchar^^d8{\v R} \gdefchar^^d9{\ringaccent U} \gdefchar^^da{\'U} \gdefchar^^db{\H U} \gdefchar^^dc{\"U} \gdefchar^^dd{\'Y} \gdefchar^^de{\cedilla T} \gdefchar^^df{\ss} % \gdefchar^^e0{\'r} \gdefchar^^e1{\'a} \gdefchar^^e2{\^a} \gdefchar^^e3{\u a} \gdefchar^^e4{\"a} \gdefchar^^e5{\'l} \gdefchar^^e6{\'c} \gdefchar^^e7{\cedilla c} \gdefchar^^e8{\v c} \gdefchar^^e9{\'e} \gdefchar^^ea{\ogonek{e}} \gdefchar^^eb{\"e} \gdefchar^^ec{\v e} \gdefchar^^ed{\'{\dotless{i}}} \gdefchar^^ee{\^{\dotless{i}}} \gdefchar^^ef{\v d} % \gdefchar^^f0{\dh} \gdefchar^^f1{\'n} \gdefchar^^f2{\v n} \gdefchar^^f3{\'o} \gdefchar^^f4{\^o} \gdefchar^^f5{\H o} \gdefchar^^f6{\"o} \gdefchar^^f7{$\div$} \gdefchar^^f8{\v r} \gdefchar^^f9{\ringaccent u} \gdefchar^^fa{\'u} \gdefchar^^fb{\H u} \gdefchar^^fc{\"u} \gdefchar^^fd{\'y} \gdefchar^^fe{\cedilla t} \gdefchar^^ff{\dotaccent{}} } % UTF-8 character definitions. % % This code to support UTF-8 is based on LaTeX's utf8.def, with some % changes for Texinfo conventions. It is included here under the GPL by % permission from Frank Mittelbach and the LaTeX team. % \newcount\countUTFx \newcount\countUTFy \newcount\countUTFz \gdef\UTFviiiTwoOctets#1#2{\expandafter \UTFviiiDefined\csname u8:#1\string #2\endcsname} % \gdef\UTFviiiThreeOctets#1#2#3{\expandafter \UTFviiiDefined\csname u8:#1\string #2\string #3\endcsname} % \gdef\UTFviiiFourOctets#1#2#3#4{\expandafter \UTFviiiDefined\csname u8:#1\string #2\string #3\string #4\endcsname} \gdef\UTFviiiDefined#1{% \ifx #1\relax \message{\linenumber Unicode char \string #1 not defined for Texinfo}% \else \expandafter #1% \fi } % Give non-ASCII bytes the active definitions for processing UTF-8 sequences \begingroup \catcode`\~13 \catcode`\$12 \catcode`\"12 % Loop from \countUTFx to \countUTFy, performing \UTFviiiTmp % substituting ~ and $ with a character token of that value. \def\UTFviiiLoop{% \global\catcode\countUTFx\active \uccode`\~\countUTFx \uccode`\$\countUTFx \uppercase\expandafter{\UTFviiiTmp}% \advance\countUTFx by 1 \ifnum\countUTFx < \countUTFy \expandafter\UTFviiiLoop \fi} % For bytes other than the first in a UTF-8 sequence. Not expected to % be expanded except when writing to auxiliary files. \countUTFx = "80 \countUTFy = "C2 \def\UTFviiiTmp{% \gdef~{% \ifpassthroughchars $\fi}}% \UTFviiiLoop \countUTFx = "C2 \countUTFy = "E0 \def\UTFviiiTmp{% \gdef~{% \ifpassthroughchars $% \else\expandafter\UTFviiiTwoOctets\expandafter$\fi}}% \UTFviiiLoop \countUTFx = "E0 \countUTFy = "F0 \def\UTFviiiTmp{% \gdef~{% \ifpassthroughchars $% \else\expandafter\UTFviiiThreeOctets\expandafter$\fi}}% \UTFviiiLoop \countUTFx = "F0 \countUTFy = "F4 \def\UTFviiiTmp{% \gdef~{% \ifpassthroughchars $% \else\expandafter\UTFviiiFourOctets\expandafter$\fi }}% \UTFviiiLoop \endgroup \def\globallet{\global\let} % save some \expandafter's below % @U{xxxx} to produce U+xxxx, if we support it. \def\U#1{% \expandafter\ifx\csname uni:#1\endcsname \relax \iftxinativeunicodecapable % All Unicode characters can be used if native Unicode handling is % active. However, if the font does not have the glyph, % letters are missing. \begingroup \uccode`\.="#1\relax \uppercase{.} \endgroup \else \errhelp = \EMsimple \errmessage{Unicode character U+#1 not supported, sorry}% \fi \else \csname uni:#1\endcsname \fi } % These macros are used here to construct the name of a control % sequence to be defined. \def\UTFviiiTwoOctetsName#1#2{% \csname u8:#1\string #2\endcsname}% \def\UTFviiiThreeOctetsName#1#2#3{% \csname u8:#1\string #2\string #3\endcsname}% \def\UTFviiiFourOctetsName#1#2#3#4{% \csname u8:#1\string #2\string #3\string #4\endcsname}% % For UTF-8 byte sequences (TeX, e-TeX and pdfTeX), % provide a definition macro to replace a Unicode character; % this gets used by the @U command % \begingroup \catcode`\"=12 \catcode`\<=12 \catcode`\.=12 \catcode`\,=12 \catcode`\;=12 \catcode`\!=12 \catcode`\~=13 \gdef\DeclareUnicodeCharacterUTFviii#1#2{% \countUTFz = "#1\relax \begingroup \parseXMLCharref % Give \u8:... its definition. The sequence of seven \expandafter's % expands after the \gdef three times, e.g. % % 1. \UTFviiTwoOctetsName B1 B2 % 2. \csname u8:B1 \string B2 \endcsname % 3. \u8: B1 B2 (a single control sequence token) % \expandafter\expandafter \expandafter\expandafter \expandafter\expandafter \expandafter\gdef \UTFviiiTmp{#2}% % \expandafter\ifx\csname uni:#1\endcsname \relax \else \message{Internal error, already defined: #1}% \fi % % define an additional control sequence for this code point. \expandafter\globallet\csname uni:#1\endcsname \UTFviiiTmp \endgroup} % % Given the value in \countUTFz as a Unicode code point, set \UTFviiiTmp % to the corresponding UTF-8 sequence. \gdef\parseXMLCharref{% \ifnum\countUTFz < "A0\relax \errhelp = \EMsimple \errmessage{Cannot define Unicode char value < 00A0}% \else\ifnum\countUTFz < "800\relax \parseUTFviiiA,% \parseUTFviiiB C\UTFviiiTwoOctetsName.,% \else\ifnum\countUTFz < "10000\relax \parseUTFviiiA;% \parseUTFviiiA,% \parseUTFviiiB E\UTFviiiThreeOctetsName.{,;}% \else \parseUTFviiiA;% \parseUTFviiiA,% \parseUTFviiiA!% \parseUTFviiiB F\UTFviiiFourOctetsName.{!,;}% \fi\fi\fi } % Extract a byte from the end of the UTF-8 representation of \countUTFx. % It must be a non-initial byte in the sequence. % Change \uccode of #1 for it to be used in \parseUTFviiiB as one % of the bytes. \gdef\parseUTFviiiA#1{% \countUTFx = \countUTFz \divide\countUTFz by 64 \countUTFy = \countUTFz % Save to be the future value of \countUTFz. \multiply\countUTFz by 64 % \countUTFz is now \countUTFx with the last 5 bits cleared. Subtract % in order to get the last five bits. \advance\countUTFx by -\countUTFz % Convert this to the byte in the UTF-8 sequence. \advance\countUTFx by 128 \uccode `#1\countUTFx \countUTFz = \countUTFy} % Used to put a UTF-8 byte sequence into \UTFviiiTmp % #1 is the increment for \countUTFz to yield a the first byte of the UTF-8 % sequence. % #2 is one of the \UTFviii*OctetsName macros. % #3 is always a full stop (.) % #4 is a template for the other bytes in the sequence. The values for these % bytes is substituted in here with \uppercase using the \uccode's. \gdef\parseUTFviiiB#1#2#3#4{% \advance\countUTFz by "#10\relax \uccode `#3\countUTFz \uppercase{\gdef\UTFviiiTmp{#2#3#4}}} \endgroup % For native Unicode handling (XeTeX and LuaTeX), % provide a definition macro that sets a catcode to `other' non-globally % \def\DeclareUnicodeCharacterNativeOther#1#2{% \catcode"#1=\other } % https://en.wikipedia.org/wiki/Plane_(Unicode)#Basic_M % U+0000..U+007F = https://en.wikipedia.org/wiki/Basic_Latin_(Unicode_block) % U+0080..U+00FF = https://en.wikipedia.org/wiki/Latin-1_Supplement_(Unicode_block) % U+0100..U+017F = https://en.wikipedia.org/wiki/Latin_Extended-A % U+0180..U+024F = https://en.wikipedia.org/wiki/Latin_Extended-B % % Many of our renditions are less than wonderful, and all the missing % characters are available somewhere. Loading the necessary fonts % awaits user request. We can't truly support Unicode without % reimplementing everything that's been done in LaTeX for many years, % plus probably using luatex or xetex, and who knows what else. % We won't be doing that here in this simple file. But we can try to at % least make most of the characters not bomb out. % \def\unicodechardefs{% \DeclareUnicodeCharacter{00A0}{\tie}% \DeclareUnicodeCharacter{00A1}{\exclamdown}% \DeclareUnicodeCharacter{00A2}{{\tcfont \char162}}% 0242=cent \DeclareUnicodeCharacter{00A3}{\pounds{}}% \DeclareUnicodeCharacter{00A4}{{\tcfont \char164}}% 0244=currency \DeclareUnicodeCharacter{00A5}{{\tcfont \char165}}% 0245=yen \DeclareUnicodeCharacter{00A6}{{\tcfont \char166}}% 0246=brokenbar \DeclareUnicodeCharacter{00A7}{\S}% \DeclareUnicodeCharacter{00A8}{\"{ }}% \DeclareUnicodeCharacter{00A9}{\copyright{}}% \DeclareUnicodeCharacter{00AA}{\ordf}% \DeclareUnicodeCharacter{00AB}{\guillemetleft{}}% \DeclareUnicodeCharacter{00AC}{\ensuremath\lnot}% \DeclareUnicodeCharacter{00AD}{\-}% \DeclareUnicodeCharacter{00AE}{\registeredsymbol{}}% \DeclareUnicodeCharacter{00AF}{\={ }}% % \DeclareUnicodeCharacter{00B0}{\ringaccent{ }}% \DeclareUnicodeCharacter{00B1}{\ensuremath\pm}% \DeclareUnicodeCharacter{00B2}{$^2$}% \DeclareUnicodeCharacter{00B3}{$^3$}% \DeclareUnicodeCharacter{00B4}{\'{ }}% \DeclareUnicodeCharacter{00B5}{$\mu$}% \DeclareUnicodeCharacter{00B6}{\P}% \DeclareUnicodeCharacter{00B7}{\ensuremath\cdot}% \DeclareUnicodeCharacter{00B8}{\cedilla{ }}% \DeclareUnicodeCharacter{00B9}{$^1$}% \DeclareUnicodeCharacter{00BA}{\ordm}% \DeclareUnicodeCharacter{00BB}{\guillemetright{}}% \DeclareUnicodeCharacter{00BC}{$1\over4$}% \DeclareUnicodeCharacter{00BD}{$1\over2$}% \DeclareUnicodeCharacter{00BE}{$3\over4$}% \DeclareUnicodeCharacter{00BF}{\questiondown}% % \DeclareUnicodeCharacter{00C0}{\`A}% \DeclareUnicodeCharacter{00C1}{\'A}% \DeclareUnicodeCharacter{00C2}{\^A}% \DeclareUnicodeCharacter{00C3}{\~A}% \DeclareUnicodeCharacter{00C4}{\"A}% \DeclareUnicodeCharacter{00C5}{\AA}% \DeclareUnicodeCharacter{00C6}{\AE}% \DeclareUnicodeCharacter{00C7}{\cedilla{C}}% \DeclareUnicodeCharacter{00C8}{\`E}% \DeclareUnicodeCharacter{00C9}{\'E}% \DeclareUnicodeCharacter{00CA}{\^E}% \DeclareUnicodeCharacter{00CB}{\"E}% \DeclareUnicodeCharacter{00CC}{\`I}% \DeclareUnicodeCharacter{00CD}{\'I}% \DeclareUnicodeCharacter{00CE}{\^I}% \DeclareUnicodeCharacter{00CF}{\"I}% % \DeclareUnicodeCharacter{00D0}{\DH}% \DeclareUnicodeCharacter{00D1}{\~N}% \DeclareUnicodeCharacter{00D2}{\`O}% \DeclareUnicodeCharacter{00D3}{\'O}% \DeclareUnicodeCharacter{00D4}{\^O}% \DeclareUnicodeCharacter{00D5}{\~O}% \DeclareUnicodeCharacter{00D6}{\"O}% \DeclareUnicodeCharacter{00D7}{\ensuremath\times}% \DeclareUnicodeCharacter{00D8}{\O}% \DeclareUnicodeCharacter{00D9}{\`U}% \DeclareUnicodeCharacter{00DA}{\'U}% \DeclareUnicodeCharacter{00DB}{\^U}% \DeclareUnicodeCharacter{00DC}{\"U}% \DeclareUnicodeCharacter{00DD}{\'Y}% \DeclareUnicodeCharacter{00DE}{\TH}% \DeclareUnicodeCharacter{00DF}{\ss}% % \DeclareUnicodeCharacter{00E0}{\`a}% \DeclareUnicodeCharacter{00E1}{\'a}% \DeclareUnicodeCharacter{00E2}{\^a}% \DeclareUnicodeCharacter{00E3}{\~a}% \DeclareUnicodeCharacter{00E4}{\"a}% \DeclareUnicodeCharacter{00E5}{\aa}% \DeclareUnicodeCharacter{00E6}{\ae}% \DeclareUnicodeCharacter{00E7}{\cedilla{c}}% \DeclareUnicodeCharacter{00E8}{\`e}% \DeclareUnicodeCharacter{00E9}{\'e}% \DeclareUnicodeCharacter{00EA}{\^e}% \DeclareUnicodeCharacter{00EB}{\"e}% \DeclareUnicodeCharacter{00EC}{\`{\dotless{i}}}% \DeclareUnicodeCharacter{00ED}{\'{\dotless{i}}}% \DeclareUnicodeCharacter{00EE}{\^{\dotless{i}}}% \DeclareUnicodeCharacter{00EF}{\"{\dotless{i}}}% % \DeclareUnicodeCharacter{00F0}{\dh}% \DeclareUnicodeCharacter{00F1}{\~n}% \DeclareUnicodeCharacter{00F2}{\`o}% \DeclareUnicodeCharacter{00F3}{\'o}% \DeclareUnicodeCharacter{00F4}{\^o}% \DeclareUnicodeCharacter{00F5}{\~o}% \DeclareUnicodeCharacter{00F6}{\"o}% \DeclareUnicodeCharacter{00F7}{\ensuremath\div}% \DeclareUnicodeCharacter{00F8}{\o}% \DeclareUnicodeCharacter{00F9}{\`u}% \DeclareUnicodeCharacter{00FA}{\'u}% \DeclareUnicodeCharacter{00FB}{\^u}% \DeclareUnicodeCharacter{00FC}{\"u}% \DeclareUnicodeCharacter{00FD}{\'y}% \DeclareUnicodeCharacter{00FE}{\th}% \DeclareUnicodeCharacter{00FF}{\"y}% % \DeclareUnicodeCharacter{0100}{\=A}% \DeclareUnicodeCharacter{0101}{\=a}% \DeclareUnicodeCharacter{0102}{\u{A}}% \DeclareUnicodeCharacter{0103}{\u{a}}% \DeclareUnicodeCharacter{0104}{\ogonek{A}}% \DeclareUnicodeCharacter{0105}{\ogonek{a}}% \DeclareUnicodeCharacter{0106}{\'C}% \DeclareUnicodeCharacter{0107}{\'c}% \DeclareUnicodeCharacter{0108}{\^C}% \DeclareUnicodeCharacter{0109}{\^c}% \DeclareUnicodeCharacter{010A}{\dotaccent{C}}% \DeclareUnicodeCharacter{010B}{\dotaccent{c}}% \DeclareUnicodeCharacter{010C}{\v{C}}% \DeclareUnicodeCharacter{010D}{\v{c}}% \DeclareUnicodeCharacter{010E}{\v{D}}% \DeclareUnicodeCharacter{010F}{d'}% % \DeclareUnicodeCharacter{0110}{\DH}% \DeclareUnicodeCharacter{0111}{\dh}% \DeclareUnicodeCharacter{0112}{\=E}% \DeclareUnicodeCharacter{0113}{\=e}% \DeclareUnicodeCharacter{0114}{\u{E}}% \DeclareUnicodeCharacter{0115}{\u{e}}% \DeclareUnicodeCharacter{0116}{\dotaccent{E}}% \DeclareUnicodeCharacter{0117}{\dotaccent{e}}% \DeclareUnicodeCharacter{0118}{\ogonek{E}}% \DeclareUnicodeCharacter{0119}{\ogonek{e}}% \DeclareUnicodeCharacter{011A}{\v{E}}% \DeclareUnicodeCharacter{011B}{\v{e}}% \DeclareUnicodeCharacter{011C}{\^G}% \DeclareUnicodeCharacter{011D}{\^g}% \DeclareUnicodeCharacter{011E}{\u{G}}% \DeclareUnicodeCharacter{011F}{\u{g}}% % \DeclareUnicodeCharacter{0120}{\dotaccent{G}}% \DeclareUnicodeCharacter{0121}{\dotaccent{g}}% \DeclareUnicodeCharacter{0122}{\cedilla{G}}% \DeclareUnicodeCharacter{0123}{\cedilla{g}}% \DeclareUnicodeCharacter{0124}{\^H}% \DeclareUnicodeCharacter{0125}{\^h}% \DeclareUnicodeCharacter{0126}{\missingcharmsg{H WITH STROKE}}% \DeclareUnicodeCharacter{0127}{\missingcharmsg{h WITH STROKE}}% \DeclareUnicodeCharacter{0128}{\~I}% \DeclareUnicodeCharacter{0129}{\~{\dotless{i}}}% \DeclareUnicodeCharacter{012A}{\=I}% \DeclareUnicodeCharacter{012B}{\={\dotless{i}}}% \DeclareUnicodeCharacter{012C}{\u{I}}% \DeclareUnicodeCharacter{012D}{\u{\dotless{i}}}% \DeclareUnicodeCharacter{012E}{\ogonek{I}}% \DeclareUnicodeCharacter{012F}{\ogonek{i}}% % \DeclareUnicodeCharacter{0130}{\dotaccent{I}}% \DeclareUnicodeCharacter{0131}{\dotless{i}}% \DeclareUnicodeCharacter{0132}{IJ}% \DeclareUnicodeCharacter{0133}{ij}% \DeclareUnicodeCharacter{0134}{\^J}% \DeclareUnicodeCharacter{0135}{\^{\dotless{j}}}% \DeclareUnicodeCharacter{0136}{\cedilla{K}}% \DeclareUnicodeCharacter{0137}{\cedilla{k}}% \DeclareUnicodeCharacter{0138}{\ensuremath\kappa}% \DeclareUnicodeCharacter{0139}{\'L}% \DeclareUnicodeCharacter{013A}{\'l}% \DeclareUnicodeCharacter{013B}{\cedilla{L}}% \DeclareUnicodeCharacter{013C}{\cedilla{l}}% \DeclareUnicodeCharacter{013D}{L'}% should kern \DeclareUnicodeCharacter{013E}{l'}% should kern \DeclareUnicodeCharacter{013F}{L\U{00B7}}% % \DeclareUnicodeCharacter{0140}{l\U{00B7}}% \DeclareUnicodeCharacter{0141}{\L}% \DeclareUnicodeCharacter{0142}{\l}% \DeclareUnicodeCharacter{0143}{\'N}% \DeclareUnicodeCharacter{0144}{\'n}% \DeclareUnicodeCharacter{0145}{\cedilla{N}}% \DeclareUnicodeCharacter{0146}{\cedilla{n}}% \DeclareUnicodeCharacter{0147}{\v{N}}% \DeclareUnicodeCharacter{0148}{\v{n}}% \DeclareUnicodeCharacter{0149}{'n}% \DeclareUnicodeCharacter{014A}{\missingcharmsg{ENG}}% \DeclareUnicodeCharacter{014B}{\missingcharmsg{eng}}% \DeclareUnicodeCharacter{014C}{\=O}% \DeclareUnicodeCharacter{014D}{\=o}% \DeclareUnicodeCharacter{014E}{\u{O}}% \DeclareUnicodeCharacter{014F}{\u{o}}% % \DeclareUnicodeCharacter{0150}{\H{O}}% \DeclareUnicodeCharacter{0151}{\H{o}}% \DeclareUnicodeCharacter{0152}{\OE}% \DeclareUnicodeCharacter{0153}{\oe}% \DeclareUnicodeCharacter{0154}{\'R}% \DeclareUnicodeCharacter{0155}{\'r}% \DeclareUnicodeCharacter{0156}{\cedilla{R}}% \DeclareUnicodeCharacter{0157}{\cedilla{r}}% \DeclareUnicodeCharacter{0158}{\v{R}}% \DeclareUnicodeCharacter{0159}{\v{r}}% \DeclareUnicodeCharacter{015A}{\'S}% \DeclareUnicodeCharacter{015B}{\'s}% \DeclareUnicodeCharacter{015C}{\^S}% \DeclareUnicodeCharacter{015D}{\^s}% \DeclareUnicodeCharacter{015E}{\cedilla{S}}% \DeclareUnicodeCharacter{015F}{\cedilla{s}}% % \DeclareUnicodeCharacter{0160}{\v{S}}% \DeclareUnicodeCharacter{0161}{\v{s}}% \DeclareUnicodeCharacter{0162}{\cedilla{T}}% \DeclareUnicodeCharacter{0163}{\cedilla{t}}% \DeclareUnicodeCharacter{0164}{\v{T}}% \DeclareUnicodeCharacter{0165}{\v{t}}% \DeclareUnicodeCharacter{0166}{\missingcharmsg{H WITH STROKE}}% \DeclareUnicodeCharacter{0167}{\missingcharmsg{h WITH STROKE}}% \DeclareUnicodeCharacter{0168}{\~U}% \DeclareUnicodeCharacter{0169}{\~u}% \DeclareUnicodeCharacter{016A}{\=U}% \DeclareUnicodeCharacter{016B}{\=u}% \DeclareUnicodeCharacter{016C}{\u{U}}% \DeclareUnicodeCharacter{016D}{\u{u}}% \DeclareUnicodeCharacter{016E}{\ringaccent{U}}% \DeclareUnicodeCharacter{016F}{\ringaccent{u}}% % \DeclareUnicodeCharacter{0170}{\H{U}}% \DeclareUnicodeCharacter{0171}{\H{u}}% \DeclareUnicodeCharacter{0172}{\ogonek{U}}% \DeclareUnicodeCharacter{0173}{\ogonek{u}}% \DeclareUnicodeCharacter{0174}{\^W}% \DeclareUnicodeCharacter{0175}{\^w}% \DeclareUnicodeCharacter{0176}{\^Y}% \DeclareUnicodeCharacter{0177}{\^y}% \DeclareUnicodeCharacter{0178}{\"Y}% \DeclareUnicodeCharacter{0179}{\'Z}% \DeclareUnicodeCharacter{017A}{\'z}% \DeclareUnicodeCharacter{017B}{\dotaccent{Z}}% \DeclareUnicodeCharacter{017C}{\dotaccent{z}}% \DeclareUnicodeCharacter{017D}{\v{Z}}% \DeclareUnicodeCharacter{017E}{\v{z}}% \DeclareUnicodeCharacter{017F}{\missingcharmsg{LONG S}}% % \DeclareUnicodeCharacter{01C4}{D\v{Z}}% \DeclareUnicodeCharacter{01C5}{D\v{z}}% \DeclareUnicodeCharacter{01C6}{d\v{z}}% \DeclareUnicodeCharacter{01C7}{LJ}% \DeclareUnicodeCharacter{01C8}{Lj}% \DeclareUnicodeCharacter{01C9}{lj}% \DeclareUnicodeCharacter{01CA}{NJ}% \DeclareUnicodeCharacter{01CB}{Nj}% \DeclareUnicodeCharacter{01CC}{nj}% \DeclareUnicodeCharacter{01CD}{\v{A}}% \DeclareUnicodeCharacter{01CE}{\v{a}}% \DeclareUnicodeCharacter{01CF}{\v{I}}% % \DeclareUnicodeCharacter{01D0}{\v{\dotless{i}}}% \DeclareUnicodeCharacter{01D1}{\v{O}}% \DeclareUnicodeCharacter{01D2}{\v{o}}% \DeclareUnicodeCharacter{01D3}{\v{U}}% \DeclareUnicodeCharacter{01D4}{\v{u}}% % \DeclareUnicodeCharacter{01E2}{\={\AE}}% \DeclareUnicodeCharacter{01E3}{\={\ae}}% \DeclareUnicodeCharacter{01E6}{\v{G}}% \DeclareUnicodeCharacter{01E7}{\v{g}}% \DeclareUnicodeCharacter{01E8}{\v{K}}% \DeclareUnicodeCharacter{01E9}{\v{k}}% % \DeclareUnicodeCharacter{01F0}{\v{\dotless{j}}}% \DeclareUnicodeCharacter{01F1}{DZ}% \DeclareUnicodeCharacter{01F2}{Dz}% \DeclareUnicodeCharacter{01F3}{dz}% \DeclareUnicodeCharacter{01F4}{\'G}% \DeclareUnicodeCharacter{01F5}{\'g}% \DeclareUnicodeCharacter{01F8}{\`N}% \DeclareUnicodeCharacter{01F9}{\`n}% \DeclareUnicodeCharacter{01FC}{\'{\AE}}% \DeclareUnicodeCharacter{01FD}{\'{\ae}}% \DeclareUnicodeCharacter{01FE}{\'{\O}}% \DeclareUnicodeCharacter{01FF}{\'{\o}}% % \DeclareUnicodeCharacter{021E}{\v{H}}% \DeclareUnicodeCharacter{021F}{\v{h}}% % \DeclareUnicodeCharacter{0226}{\dotaccent{A}}% \DeclareUnicodeCharacter{0227}{\dotaccent{a}}% \DeclareUnicodeCharacter{0228}{\cedilla{E}}% \DeclareUnicodeCharacter{0229}{\cedilla{e}}% \DeclareUnicodeCharacter{022E}{\dotaccent{O}}% \DeclareUnicodeCharacter{022F}{\dotaccent{o}}% % \DeclareUnicodeCharacter{0232}{\=Y}% \DeclareUnicodeCharacter{0233}{\=y}% \DeclareUnicodeCharacter{0237}{\dotless{j}}% % \DeclareUnicodeCharacter{02DB}{\ogonek{ }}% % % Greek letters upper case \DeclareUnicodeCharacter{0391}{{\it A}}% \DeclareUnicodeCharacter{0392}{{\it B}}% \DeclareUnicodeCharacter{0393}{\ensuremath{\mit\Gamma}}% \DeclareUnicodeCharacter{0394}{\ensuremath{\mit\Delta}}% \DeclareUnicodeCharacter{0395}{{\it E}}% \DeclareUnicodeCharacter{0396}{{\it Z}}% \DeclareUnicodeCharacter{0397}{{\it H}}% \DeclareUnicodeCharacter{0398}{\ensuremath{\mit\Theta}}% \DeclareUnicodeCharacter{0399}{{\it I}}% \DeclareUnicodeCharacter{039A}{{\it K}}% \DeclareUnicodeCharacter{039B}{\ensuremath{\mit\Lambda}}% \DeclareUnicodeCharacter{039C}{{\it M}}% \DeclareUnicodeCharacter{039D}{{\it N}}% \DeclareUnicodeCharacter{039E}{\ensuremath{\mit\Xi}}% \DeclareUnicodeCharacter{039F}{{\it O}}% \DeclareUnicodeCharacter{03A0}{\ensuremath{\mit\Pi}}% \DeclareUnicodeCharacter{03A1}{{\it P}}% %\DeclareUnicodeCharacter{03A2}{} % none - corresponds to final sigma \DeclareUnicodeCharacter{03A3}{\ensuremath{\mit\Sigma}}% \DeclareUnicodeCharacter{03A4}{{\it T}}% \DeclareUnicodeCharacter{03A5}{\ensuremath{\mit\Upsilon}}% \DeclareUnicodeCharacter{03A6}{\ensuremath{\mit\Phi}}% \DeclareUnicodeCharacter{03A7}{{\it X}}% \DeclareUnicodeCharacter{03A8}{\ensuremath{\mit\Psi}}% \DeclareUnicodeCharacter{03A9}{\ensuremath{\mit\Omega}}% % % Vowels with accents \DeclareUnicodeCharacter{0390}{\ensuremath{\ddot{\acute\iota}}}% \DeclareUnicodeCharacter{03AC}{\ensuremath{\acute\alpha}}% \DeclareUnicodeCharacter{03AD}{\ensuremath{\acute\epsilon}}% \DeclareUnicodeCharacter{03AE}{\ensuremath{\acute\eta}}% \DeclareUnicodeCharacter{03AF}{\ensuremath{\acute\iota}}% \DeclareUnicodeCharacter{03B0}{\ensuremath{\acute{\ddot\upsilon}}}% % % Standalone accent \DeclareUnicodeCharacter{0384}{\ensuremath{\acute{\ }}}% % % Greek letters lower case \DeclareUnicodeCharacter{03B1}{\ensuremath\alpha}% \DeclareUnicodeCharacter{03B2}{\ensuremath\beta}% \DeclareUnicodeCharacter{03B3}{\ensuremath\gamma}% \DeclareUnicodeCharacter{03B4}{\ensuremath\delta}% \DeclareUnicodeCharacter{03B5}{\ensuremath\epsilon}% \DeclareUnicodeCharacter{03B6}{\ensuremath\zeta}% \DeclareUnicodeCharacter{03B7}{\ensuremath\eta}% \DeclareUnicodeCharacter{03B8}{\ensuremath\theta}% \DeclareUnicodeCharacter{03B9}{\ensuremath\iota}% \DeclareUnicodeCharacter{03BA}{\ensuremath\kappa}% \DeclareUnicodeCharacter{03BB}{\ensuremath\lambda}% \DeclareUnicodeCharacter{03BC}{\ensuremath\mu}% \DeclareUnicodeCharacter{03BD}{\ensuremath\nu}% \DeclareUnicodeCharacter{03BE}{\ensuremath\xi}% \DeclareUnicodeCharacter{03BF}{{\it o}}% omicron \DeclareUnicodeCharacter{03C0}{\ensuremath\pi}% \DeclareUnicodeCharacter{03C1}{\ensuremath\rho}% \DeclareUnicodeCharacter{03C2}{\ensuremath\varsigma}% \DeclareUnicodeCharacter{03C3}{\ensuremath\sigma}% \DeclareUnicodeCharacter{03C4}{\ensuremath\tau}% \DeclareUnicodeCharacter{03C5}{\ensuremath\upsilon}% \DeclareUnicodeCharacter{03C6}{\ensuremath\phi}% \DeclareUnicodeCharacter{03C7}{\ensuremath\chi}% \DeclareUnicodeCharacter{03C8}{\ensuremath\psi}% \DeclareUnicodeCharacter{03C9}{\ensuremath\omega}% % % More Greek vowels with accents \DeclareUnicodeCharacter{03CA}{\ensuremath{\ddot\iota}}% \DeclareUnicodeCharacter{03CB}{\ensuremath{\ddot\upsilon}}% \DeclareUnicodeCharacter{03CC}{\ensuremath{\acute o}}% \DeclareUnicodeCharacter{03CD}{\ensuremath{\acute\upsilon}}% \DeclareUnicodeCharacter{03CE}{\ensuremath{\acute\omega}}% % % Variant Greek letters \DeclareUnicodeCharacter{03D1}{\ensuremath\vartheta}% \DeclareUnicodeCharacter{03D6}{\ensuremath\varpi}% \DeclareUnicodeCharacter{03F1}{\ensuremath\varrho}% % \DeclareUnicodeCharacter{1E02}{\dotaccent{B}}% \DeclareUnicodeCharacter{1E03}{\dotaccent{b}}% \DeclareUnicodeCharacter{1E04}{\udotaccent{B}}% \DeclareUnicodeCharacter{1E05}{\udotaccent{b}}% \DeclareUnicodeCharacter{1E06}{\ubaraccent{B}}% \DeclareUnicodeCharacter{1E07}{\ubaraccent{b}}% \DeclareUnicodeCharacter{1E0A}{\dotaccent{D}}% \DeclareUnicodeCharacter{1E0B}{\dotaccent{d}}% \DeclareUnicodeCharacter{1E0C}{\udotaccent{D}}% \DeclareUnicodeCharacter{1E0D}{\udotaccent{d}}% \DeclareUnicodeCharacter{1E0E}{\ubaraccent{D}}% \DeclareUnicodeCharacter{1E0F}{\ubaraccent{d}}% % \DeclareUnicodeCharacter{1E1E}{\dotaccent{F}}% \DeclareUnicodeCharacter{1E1F}{\dotaccent{f}}% % \DeclareUnicodeCharacter{1E20}{\=G}% \DeclareUnicodeCharacter{1E21}{\=g}% \DeclareUnicodeCharacter{1E22}{\dotaccent{H}}% \DeclareUnicodeCharacter{1E23}{\dotaccent{h}}% \DeclareUnicodeCharacter{1E24}{\udotaccent{H}}% \DeclareUnicodeCharacter{1E25}{\udotaccent{h}}% \DeclareUnicodeCharacter{1E26}{\"H}% \DeclareUnicodeCharacter{1E27}{\"h}% % \DeclareUnicodeCharacter{1E30}{\'K}% \DeclareUnicodeCharacter{1E31}{\'k}% \DeclareUnicodeCharacter{1E32}{\udotaccent{K}}% \DeclareUnicodeCharacter{1E33}{\udotaccent{k}}% \DeclareUnicodeCharacter{1E34}{\ubaraccent{K}}% \DeclareUnicodeCharacter{1E35}{\ubaraccent{k}}% \DeclareUnicodeCharacter{1E36}{\udotaccent{L}}% \DeclareUnicodeCharacter{1E37}{\udotaccent{l}}% \DeclareUnicodeCharacter{1E3A}{\ubaraccent{L}}% \DeclareUnicodeCharacter{1E3B}{\ubaraccent{l}}% \DeclareUnicodeCharacter{1E3E}{\'M}% \DeclareUnicodeCharacter{1E3F}{\'m}% % \DeclareUnicodeCharacter{1E40}{\dotaccent{M}}% \DeclareUnicodeCharacter{1E41}{\dotaccent{m}}% \DeclareUnicodeCharacter{1E42}{\udotaccent{M}}% \DeclareUnicodeCharacter{1E43}{\udotaccent{m}}% \DeclareUnicodeCharacter{1E44}{\dotaccent{N}}% \DeclareUnicodeCharacter{1E45}{\dotaccent{n}}% \DeclareUnicodeCharacter{1E46}{\udotaccent{N}}% \DeclareUnicodeCharacter{1E47}{\udotaccent{n}}% \DeclareUnicodeCharacter{1E48}{\ubaraccent{N}}% \DeclareUnicodeCharacter{1E49}{\ubaraccent{n}}% % \DeclareUnicodeCharacter{1E54}{\'P}% \DeclareUnicodeCharacter{1E55}{\'p}% \DeclareUnicodeCharacter{1E56}{\dotaccent{P}}% \DeclareUnicodeCharacter{1E57}{\dotaccent{p}}% \DeclareUnicodeCharacter{1E58}{\dotaccent{R}}% \DeclareUnicodeCharacter{1E59}{\dotaccent{r}}% \DeclareUnicodeCharacter{1E5A}{\udotaccent{R}}% \DeclareUnicodeCharacter{1E5B}{\udotaccent{r}}% \DeclareUnicodeCharacter{1E5E}{\ubaraccent{R}}% \DeclareUnicodeCharacter{1E5F}{\ubaraccent{r}}% % \DeclareUnicodeCharacter{1E60}{\dotaccent{S}}% \DeclareUnicodeCharacter{1E61}{\dotaccent{s}}% \DeclareUnicodeCharacter{1E62}{\udotaccent{S}}% \DeclareUnicodeCharacter{1E63}{\udotaccent{s}}% \DeclareUnicodeCharacter{1E6A}{\dotaccent{T}}% \DeclareUnicodeCharacter{1E6B}{\dotaccent{t}}% \DeclareUnicodeCharacter{1E6C}{\udotaccent{T}}% \DeclareUnicodeCharacter{1E6D}{\udotaccent{t}}% \DeclareUnicodeCharacter{1E6E}{\ubaraccent{T}}% \DeclareUnicodeCharacter{1E6F}{\ubaraccent{t}}% % \DeclareUnicodeCharacter{1E7C}{\~V}% \DeclareUnicodeCharacter{1E7D}{\~v}% \DeclareUnicodeCharacter{1E7E}{\udotaccent{V}}% \DeclareUnicodeCharacter{1E7F}{\udotaccent{v}}% % \DeclareUnicodeCharacter{1E80}{\`W}% \DeclareUnicodeCharacter{1E81}{\`w}% \DeclareUnicodeCharacter{1E82}{\'W}% \DeclareUnicodeCharacter{1E83}{\'w}% \DeclareUnicodeCharacter{1E84}{\"W}% \DeclareUnicodeCharacter{1E85}{\"w}% \DeclareUnicodeCharacter{1E86}{\dotaccent{W}}% \DeclareUnicodeCharacter{1E87}{\dotaccent{w}}% \DeclareUnicodeCharacter{1E88}{\udotaccent{W}}% \DeclareUnicodeCharacter{1E89}{\udotaccent{w}}% \DeclareUnicodeCharacter{1E8A}{\dotaccent{X}}% \DeclareUnicodeCharacter{1E8B}{\dotaccent{x}}% \DeclareUnicodeCharacter{1E8C}{\"X}% \DeclareUnicodeCharacter{1E8D}{\"x}% \DeclareUnicodeCharacter{1E8E}{\dotaccent{Y}}% \DeclareUnicodeCharacter{1E8F}{\dotaccent{y}}% % \DeclareUnicodeCharacter{1E90}{\^Z}% \DeclareUnicodeCharacter{1E91}{\^z}% \DeclareUnicodeCharacter{1E92}{\udotaccent{Z}}% \DeclareUnicodeCharacter{1E93}{\udotaccent{z}}% \DeclareUnicodeCharacter{1E94}{\ubaraccent{Z}}% \DeclareUnicodeCharacter{1E95}{\ubaraccent{z}}% \DeclareUnicodeCharacter{1E96}{\ubaraccent{h}}% \DeclareUnicodeCharacter{1E97}{\"t}% \DeclareUnicodeCharacter{1E98}{\ringaccent{w}}% \DeclareUnicodeCharacter{1E99}{\ringaccent{y}}% % \DeclareUnicodeCharacter{1EA0}{\udotaccent{A}}% \DeclareUnicodeCharacter{1EA1}{\udotaccent{a}}% % \DeclareUnicodeCharacter{1EB8}{\udotaccent{E}}% \DeclareUnicodeCharacter{1EB9}{\udotaccent{e}}% \DeclareUnicodeCharacter{1EBC}{\~E}% \DeclareUnicodeCharacter{1EBD}{\~e}% % \DeclareUnicodeCharacter{1ECA}{\udotaccent{I}}% \DeclareUnicodeCharacter{1ECB}{\udotaccent{i}}% \DeclareUnicodeCharacter{1ECC}{\udotaccent{O}}% \DeclareUnicodeCharacter{1ECD}{\udotaccent{o}}% % \DeclareUnicodeCharacter{1EE4}{\udotaccent{U}}% \DeclareUnicodeCharacter{1EE5}{\udotaccent{u}}% % \DeclareUnicodeCharacter{1EF2}{\`Y}% \DeclareUnicodeCharacter{1EF3}{\`y}% \DeclareUnicodeCharacter{1EF4}{\udotaccent{Y}}% % \DeclareUnicodeCharacter{1EF8}{\~Y}% \DeclareUnicodeCharacter{1EF9}{\~y}% % % Punctuation \DeclareUnicodeCharacter{2013}{--}% \DeclareUnicodeCharacter{2014}{---}% \DeclareUnicodeCharacter{2018}{\quoteleft{}}% \DeclareUnicodeCharacter{2019}{\quoteright{}}% \DeclareUnicodeCharacter{201A}{\quotesinglbase{}}% \DeclareUnicodeCharacter{201C}{\quotedblleft{}}% \DeclareUnicodeCharacter{201D}{\quotedblright{}}% \DeclareUnicodeCharacter{201E}{\quotedblbase{}}% \DeclareUnicodeCharacter{2020}{\ensuremath\dagger}% \DeclareUnicodeCharacter{2021}{\ensuremath\ddagger}% \DeclareUnicodeCharacter{2022}{\bullet{}}% \DeclareUnicodeCharacter{202F}{\thinspace}% \DeclareUnicodeCharacter{2026}{\dots{}}% \DeclareUnicodeCharacter{2039}{\guilsinglleft{}}% \DeclareUnicodeCharacter{203A}{\guilsinglright{}}% % \DeclareUnicodeCharacter{20AC}{\euro{}}% % \DeclareUnicodeCharacter{2192}{\expansion{}}% \DeclareUnicodeCharacter{21D2}{\result{}}% % % Mathematical symbols \DeclareUnicodeCharacter{2200}{\ensuremath\forall}% \DeclareUnicodeCharacter{2203}{\ensuremath\exists}% \DeclareUnicodeCharacter{2208}{\ensuremath\in}% \DeclareUnicodeCharacter{2212}{\minus{}}% \DeclareUnicodeCharacter{2217}{\ast}% \DeclareUnicodeCharacter{221E}{\ensuremath\infty}% \DeclareUnicodeCharacter{2225}{\ensuremath\parallel}% \DeclareUnicodeCharacter{2227}{\ensuremath\wedge}% \DeclareUnicodeCharacter{2229}{\ensuremath\cap}% \DeclareUnicodeCharacter{2261}{\equiv{}}% \DeclareUnicodeCharacter{2264}{\ensuremath\leq}% \DeclareUnicodeCharacter{2265}{\ensuremath\geq}% \DeclareUnicodeCharacter{2282}{\ensuremath\subset}% \DeclareUnicodeCharacter{2287}{\ensuremath\supseteq}% % \DeclareUnicodeCharacter{2016}{\ensuremath\Vert}% \DeclareUnicodeCharacter{2032}{\ensuremath\prime}% \DeclareUnicodeCharacter{210F}{\ensuremath\hbar}% \DeclareUnicodeCharacter{2111}{\ensuremath\Im}% \DeclareUnicodeCharacter{2113}{\ensuremath\ell}% \DeclareUnicodeCharacter{2118}{\ensuremath\wp}% \DeclareUnicodeCharacter{211C}{\ensuremath\Re}% \DeclareUnicodeCharacter{2127}{\ensuremath\mho}% \DeclareUnicodeCharacter{2135}{\ensuremath\aleph}% \DeclareUnicodeCharacter{2190}{\ensuremath\leftarrow}% \DeclareUnicodeCharacter{2191}{\ensuremath\uparrow}% \DeclareUnicodeCharacter{2193}{\ensuremath\downarrow}% \DeclareUnicodeCharacter{2194}{\ensuremath\leftrightarrow}% \DeclareUnicodeCharacter{2195}{\ensuremath\updownarrow}% \DeclareUnicodeCharacter{2196}{\ensuremath\nwarrow}% \DeclareUnicodeCharacter{2197}{\ensuremath\nearrow}% \DeclareUnicodeCharacter{2198}{\ensuremath\searrow}% \DeclareUnicodeCharacter{2199}{\ensuremath\swarrow}% \DeclareUnicodeCharacter{21A6}{\ensuremath\mapsto}% \DeclareUnicodeCharacter{21A9}{\ensuremath\hookleftarrow}% \DeclareUnicodeCharacter{21AA}{\ensuremath\hookrightarrow}% \DeclareUnicodeCharacter{21BC}{\ensuremath\leftharpoonup}% \DeclareUnicodeCharacter{21BD}{\ensuremath\leftharpoondown}% \DeclareUnicodeCharacter{21BE}{\ensuremath\upharpoonright}% \DeclareUnicodeCharacter{21C0}{\ensuremath\rightharpoonup}% \DeclareUnicodeCharacter{21C1}{\ensuremath\rightharpoondown}% \DeclareUnicodeCharacter{21CC}{\ensuremath\rightleftharpoons}% \DeclareUnicodeCharacter{21D0}{\ensuremath\Leftarrow}% \DeclareUnicodeCharacter{21D1}{\ensuremath\Uparrow}% \DeclareUnicodeCharacter{21D3}{\ensuremath\Downarrow}% \DeclareUnicodeCharacter{21D4}{\ensuremath\Leftrightarrow}% \DeclareUnicodeCharacter{21D5}{\ensuremath\Updownarrow}% \DeclareUnicodeCharacter{21DD}{\ensuremath\leadsto}% \DeclareUnicodeCharacter{2201}{\ensuremath\complement}% \DeclareUnicodeCharacter{2202}{\ensuremath\partial}% \DeclareUnicodeCharacter{2205}{\ensuremath\emptyset}% \DeclareUnicodeCharacter{2207}{\ensuremath\nabla}% \DeclareUnicodeCharacter{2209}{\ensuremath\notin}% \DeclareUnicodeCharacter{220B}{\ensuremath\owns}% \DeclareUnicodeCharacter{220F}{\ensuremath\prod}% \DeclareUnicodeCharacter{2210}{\ensuremath\coprod}% \DeclareUnicodeCharacter{2211}{\ensuremath\sum}% \DeclareUnicodeCharacter{2213}{\ensuremath\mp}% \DeclareUnicodeCharacter{2218}{\ensuremath\circ}% \DeclareUnicodeCharacter{221A}{\ensuremath\surd}% \DeclareUnicodeCharacter{221D}{\ensuremath\propto}% \DeclareUnicodeCharacter{2220}{\ensuremath\angle}% \DeclareUnicodeCharacter{2223}{\ensuremath\mid}% \DeclareUnicodeCharacter{2228}{\ensuremath\vee}% \DeclareUnicodeCharacter{222A}{\ensuremath\cup}% \DeclareUnicodeCharacter{222B}{\ensuremath\smallint}% \DeclareUnicodeCharacter{222E}{\ensuremath\oint}% \DeclareUnicodeCharacter{223C}{\ensuremath\sim}% \DeclareUnicodeCharacter{2240}{\ensuremath\wr}% \DeclareUnicodeCharacter{2243}{\ensuremath\simeq}% \DeclareUnicodeCharacter{2245}{\ensuremath\cong}% \DeclareUnicodeCharacter{2248}{\ensuremath\approx}% \DeclareUnicodeCharacter{224D}{\ensuremath\asymp}% \DeclareUnicodeCharacter{2250}{\ensuremath\doteq}% \DeclareUnicodeCharacter{2260}{\ensuremath\neq}% \DeclareUnicodeCharacter{226A}{\ensuremath\ll}% \DeclareUnicodeCharacter{226B}{\ensuremath\gg}% \DeclareUnicodeCharacter{227A}{\ensuremath\prec}% \DeclareUnicodeCharacter{227B}{\ensuremath\succ}% \DeclareUnicodeCharacter{2283}{\ensuremath\supset}% \DeclareUnicodeCharacter{2286}{\ensuremath\subseteq}% \DeclareUnicodeCharacter{228E}{\ensuremath\uplus}% \DeclareUnicodeCharacter{228F}{\ensuremath\sqsubset}% \DeclareUnicodeCharacter{2290}{\ensuremath\sqsupset}% \DeclareUnicodeCharacter{2291}{\ensuremath\sqsubseteq}% \DeclareUnicodeCharacter{2292}{\ensuremath\sqsupseteq}% \DeclareUnicodeCharacter{2293}{\ensuremath\sqcap}% \DeclareUnicodeCharacter{2294}{\ensuremath\sqcup}% \DeclareUnicodeCharacter{2295}{\ensuremath\oplus}% \DeclareUnicodeCharacter{2296}{\ensuremath\ominus}% \DeclareUnicodeCharacter{2297}{\ensuremath\otimes}% \DeclareUnicodeCharacter{2298}{\ensuremath\oslash}% \DeclareUnicodeCharacter{2299}{\ensuremath\odot}% \DeclareUnicodeCharacter{22A2}{\ensuremath\vdash}% \DeclareUnicodeCharacter{22A3}{\ensuremath\dashv}% \DeclareUnicodeCharacter{22A4}{\ensuremath\ptextop}% \DeclareUnicodeCharacter{22A5}{\ensuremath\bot}% \DeclareUnicodeCharacter{22A8}{\ensuremath\models}% \DeclareUnicodeCharacter{22B4}{\ensuremath\unlhd}% \DeclareUnicodeCharacter{22B5}{\ensuremath\unrhd}% \DeclareUnicodeCharacter{22C0}{\ensuremath\bigwedge}% \DeclareUnicodeCharacter{22C1}{\ensuremath\bigvee}% \DeclareUnicodeCharacter{22C2}{\ensuremath\bigcap}% \DeclareUnicodeCharacter{22C3}{\ensuremath\bigcup}% \DeclareUnicodeCharacter{22C4}{\ensuremath\diamond}% \DeclareUnicodeCharacter{22C5}{\ensuremath\cdot}% \DeclareUnicodeCharacter{22C6}{\ensuremath\star}% \DeclareUnicodeCharacter{22C8}{\ensuremath\bowtie}% \DeclareUnicodeCharacter{2308}{\ensuremath\lceil}% \DeclareUnicodeCharacter{2309}{\ensuremath\rceil}% \DeclareUnicodeCharacter{230A}{\ensuremath\lfloor}% \DeclareUnicodeCharacter{230B}{\ensuremath\rfloor}% \DeclareUnicodeCharacter{2322}{\ensuremath\frown}% \DeclareUnicodeCharacter{2323}{\ensuremath\smile}% % \DeclareUnicodeCharacter{25A1}{\ensuremath\Box}% \DeclareUnicodeCharacter{25B3}{\ensuremath\triangle}% \DeclareUnicodeCharacter{25B7}{\ensuremath\triangleright}% \DeclareUnicodeCharacter{25BD}{\ensuremath\bigtriangledown}% \DeclareUnicodeCharacter{25C1}{\ensuremath\triangleleft}% \DeclareUnicodeCharacter{25C7}{\ensuremath\Diamond}% \DeclareUnicodeCharacter{2660}{\ensuremath\spadesuit}% \DeclareUnicodeCharacter{2661}{\ensuremath\heartsuit}% \DeclareUnicodeCharacter{2662}{\ensuremath\diamondsuit}% \DeclareUnicodeCharacter{2663}{\ensuremath\clubsuit}% \DeclareUnicodeCharacter{266D}{\ensuremath\flat}% \DeclareUnicodeCharacter{266E}{\ensuremath\natural}% \DeclareUnicodeCharacter{266F}{\ensuremath\sharp}% \DeclareUnicodeCharacter{26AA}{\ensuremath\bigcirc}% \DeclareUnicodeCharacter{27B9}{\ensuremath\rangle}% \DeclareUnicodeCharacter{27C2}{\ensuremath\perp}% \DeclareUnicodeCharacter{27E8}{\ensuremath\langle}% \DeclareUnicodeCharacter{27F5}{\ensuremath\longleftarrow}% \DeclareUnicodeCharacter{27F6}{\ensuremath\longrightarrow}% \DeclareUnicodeCharacter{27F7}{\ensuremath\longleftrightarrow}% \DeclareUnicodeCharacter{27FC}{\ensuremath\longmapsto}% \DeclareUnicodeCharacter{29F5}{\ensuremath\setminus}% \DeclareUnicodeCharacter{2A00}{\ensuremath\bigodot}% \DeclareUnicodeCharacter{2A01}{\ensuremath\bigoplus}% \DeclareUnicodeCharacter{2A02}{\ensuremath\bigotimes}% \DeclareUnicodeCharacter{2A04}{\ensuremath\biguplus}% \DeclareUnicodeCharacter{2A06}{\ensuremath\bigsqcup}% \DeclareUnicodeCharacter{2A1D}{\ensuremath\Join}% \DeclareUnicodeCharacter{2A3F}{\ensuremath\amalg}% \DeclareUnicodeCharacter{2AAF}{\ensuremath\preceq}% \DeclareUnicodeCharacter{2AB0}{\ensuremath\succeq}% % \global\mathchardef\checkmark="1370% actually the square root sign \DeclareUnicodeCharacter{2713}{\ensuremath\checkmark}% }% end of \unicodechardefs % UTF-8 byte sequence (pdfTeX) definitions (replacing and @U command) % It makes the setting that replace UTF-8 byte sequence. \def\utfeightchardefs{% \let\DeclareUnicodeCharacter\DeclareUnicodeCharacterUTFviii \unicodechardefs } % Whether the active definitions of non-ASCII characters expand to % non-active tokens with the same character code. This is used to % write characters literally, instead of using active definitions for % printing the correct glyphs. \newif\ifpassthroughchars \passthroughcharsfalse % For native Unicode handling (XeTeX and LuaTeX), % provide a definition macro to replace/pass-through a Unicode character % \def\DeclareUnicodeCharacterNative#1#2{% \catcode"#1=\active \def\dodeclareunicodecharacternative##1##2##3{% \begingroup \uccode`\~="##2\relax \uppercase{\gdef~}{% \ifpassthroughchars ##1% \else ##3% \fi } \endgroup } \begingroup \uccode`\.="#1\relax \uppercase{\def\UTFNativeTmp{.}}% \expandafter\dodeclareunicodecharacternative\UTFNativeTmp{#1}{#2}% \endgroup } % Native Unicode handling (XeTeX and LuaTeX) character replacing definition. % It activates the setting that replaces Unicode characters. \def\nativeunicodechardefs{% \let\DeclareUnicodeCharacter\DeclareUnicodeCharacterNative \unicodechardefs } % For native Unicode handling (XeTeX and LuaTeX), % make the character token expand % to the sequences given in \unicodechardefs for printing. \def\DeclareUnicodeCharacterNativeAtU#1#2{% \def\UTFAtUTmp{#2} \expandafter\globallet\csname uni:#1\endcsname \UTFAtUTmp } % @U command definitions for native Unicode handling (XeTeX and LuaTeX). \def\nativeunicodechardefsatu{% \let\DeclareUnicodeCharacter\DeclareUnicodeCharacterNativeAtU \unicodechardefs } % US-ASCII character definitions. \def\asciichardefs{% nothing need be done \relax } % define all Unicode characters we know about, for the sake of @U. \iftxinativeunicodecapable \nativeunicodechardefsatu \else \utfeightchardefs \fi % Make non-ASCII characters printable again for compatibility with % existing Texinfo documents that may use them, even without declaring a % document encoding. % \setnonasciicharscatcode \other \message{formatting,} \newdimen\defaultparindent \defaultparindent = 15pt \chapheadingskip = 15pt plus 4pt minus 2pt \secheadingskip = 12pt plus 3pt minus 2pt \subsecheadingskip = 9pt plus 2pt minus 2pt % Prevent underfull vbox error messages. \vbadness = 10000 % Don't be very finicky about underfull hboxes, either. \hbadness = 6666 % Following George Bush, get rid of widows and orphans. \widowpenalty=10000 \clubpenalty=10000 % Use TeX 3.0's \emergencystretch to help line breaking, but if we're % using an old version of TeX, don't do anything. We want the amount of % stretch added to depend on the line length, hence the dependence on % \hsize. We call this whenever the paper size is set. % \def\setemergencystretch{% \ifx\emergencystretch\thisisundefined % Allow us to assign to \emergencystretch anyway. \def\emergencystretch{\dimen0}% \else \emergencystretch = .15\hsize \fi } % Parameters in order: 1) textheight; 2) textwidth; % 3) voffset; 4) hoffset; 5) binding offset; 6) topskip; % 7) physical page height; 8) physical page width. % % We also call \setleading{\textleading}, so the caller should define % \textleading. The caller should also set \parskip. % \def\internalpagesizes#1#2#3#4#5#6#7#8{% \voffset = #3\relax \topskip = #6\relax \splittopskip = \topskip % \vsize = #1\relax \advance\vsize by \topskip \outervsize = \vsize \advance\outervsize by 2\topandbottommargin \txipageheight = \vsize % \hsize = #2\relax \outerhsize = \hsize \advance\outerhsize by 0.5in \txipagewidth = \hsize % \normaloffset = #4\relax \bindingoffset = #5\relax % \ifpdf \pdfpageheight #7\relax \pdfpagewidth #8\relax % if we don't reset these, they will remain at "1 true in" of % whatever layout pdftex was dumped with. \pdfhorigin = 1 true in \pdfvorigin = 1 true in \else \ifx\XeTeXrevision\thisisundefined \else \pdfpageheight #7\relax \pdfpagewidth #8\relax % XeTeX does not have \pdfhorigin and \pdfvorigin. \fi \fi % \setleading{\textleading} % \parindent = \defaultparindent \setemergencystretch } % @letterpaper (the default). \def\letterpaper{{\globaldefs = 1 \parskip = 3pt plus 2pt minus 1pt \textleading = 13.2pt % % If page is nothing but text, make it come out even. \internalpagesizes{607.2pt}{6in}% that's 46 lines {\voffset}{.25in}% {\bindingoffset}{36pt}% {11in}{8.5in}% }} % Use @smallbook to reset parameters for 7x9.25 trim size. \def\smallbook{{\globaldefs = 1 \parskip = 2pt plus 1pt \textleading = 12pt % \internalpagesizes{7.5in}{5in}% {-.2in}{0in}% {\bindingoffset}{16pt}% {9.25in}{7in}% % \lispnarrowing = 0.3in \tolerance = 700 \hfuzz = 1pt \contentsrightmargin = 0pt \defbodyindent = .5cm }} % Use @smallerbook to reset parameters for 6x9 trim size. % (Just testing, parameters still in flux.) \def\smallerbook{{\globaldefs = 1 \parskip = 1.5pt plus 1pt \textleading = 12pt % \internalpagesizes{7.4in}{4.8in}% {-.2in}{-.4in}% {0pt}{14pt}% {9in}{6in}% % \lispnarrowing = 0.25in \tolerance = 700 \hfuzz = 1pt \contentsrightmargin = 0pt \defbodyindent = .4cm }} % Use @afourpaper to print on European A4 paper. \def\afourpaper{{\globaldefs = 1 \parskip = 3pt plus 2pt minus 1pt \textleading = 13.2pt % % Double-side printing via postscript on Laserjet 4050 % prints double-sided nicely when \bindingoffset=10mm and \hoffset=-6mm. % To change the settings for a different printer or situation, adjust % \normaloffset until the front-side and back-side texts align. Then % do the same for \bindingoffset. You can set these for testing in % your texinfo source file like this: % @tex % \global\normaloffset = -6mm % \global\bindingoffset = 10mm % @end tex \internalpagesizes{673.2pt}{160mm}% that's 51 lines {\voffset}{\hoffset}% {\bindingoffset}{44pt}% {297mm}{210mm}% % \tolerance = 700 \hfuzz = 1pt \contentsrightmargin = 0pt \defbodyindent = 5mm }} % Use @afivepaper to print on European A5 paper. % From romildo@urano.iceb.ufop.br, 2 July 2000. % He also recommends making @example and @lisp be small. \def\afivepaper{{\globaldefs = 1 \parskip = 2pt plus 1pt minus 0.1pt \textleading = 12.5pt % \internalpagesizes{160mm}{120mm}% {\voffset}{\hoffset}% {\bindingoffset}{8pt}% {210mm}{148mm}% % \lispnarrowing = 0.2in \tolerance = 800 \hfuzz = 1.2pt \contentsrightmargin = 0pt \defbodyindent = 2mm \tableindent = 12mm }} % A specific text layout, 24x15cm overall, intended for A4 paper. \def\afourlatex{{\globaldefs = 1 \afourpaper \internalpagesizes{237mm}{150mm}% {\voffset}{4.6mm}% {\bindingoffset}{7mm}% {297mm}{210mm}% % % Must explicitly reset to 0 because we call \afourpaper. \globaldefs = 0 }} % Use @afourwide to print on A4 paper in landscape format. \def\afourwide{{\globaldefs = 1 \afourpaper \internalpagesizes{241mm}{165mm}% {\voffset}{-2.95mm}% {\bindingoffset}{7mm}% {297mm}{210mm}% \globaldefs = 0 }} % @pagesizes TEXTHEIGHT[,TEXTWIDTH] % Perhaps we should allow setting the margins, \topskip, \parskip, % and/or leading, also. Or perhaps we should compute them somehow. % \parseargdef\pagesizes{\pagesizesyyy #1,,\finish} \def\pagesizesyyy#1,#2,#3\finish{{% \setbox0 = \hbox{\ignorespaces #2}\ifdim\wd0 > 0pt \hsize=#2\relax \fi \globaldefs = 1 % \parskip = 3pt plus 2pt minus 1pt \setleading{\textleading}% % \dimen0 = #1\relax \advance\dimen0 by \voffset % \dimen2 = \hsize \advance\dimen2 by \normaloffset % \internalpagesizes{#1}{\hsize}% {\voffset}{\normaloffset}% {\bindingoffset}{44pt}% {\dimen0}{\dimen2}% }} % Set default to letter. % \letterpaper \message{and turning on texinfo input format.} \def^^L{\par} % remove \outer, so ^L can appear in an @comment % DEL is a comment character, in case @c does not suffice. \catcode`\^^? = 14 % Define macros to output various characters with catcode for normal text. \catcode`\"=\other \def\normaldoublequote{"} \catcode`\$=\other \def\normaldollar{$}%$ font-lock fix \catcode`\+=\other \def\normalplus{+} \catcode`\<=\other \def\normalless{<} \catcode`\>=\other \def\normalgreater{>} \catcode`\^=\other \def\normalcaret{^} \catcode`\_=\other \def\normalunderscore{_} \catcode`\|=\other \def\normalverticalbar{|} \catcode`\~=\other \def\normaltilde{~} % This macro is used to make a character print one way in \tt % (where it can probably be output as-is), and another way in other fonts, % where something hairier probably needs to be done. % % #1 is what to print if we are indeed using \tt; #2 is what to print % otherwise. Since all the Computer Modern typewriter fonts have zero % interword stretch (and shrink), and it is reasonable to expect all % typewriter fonts to have this, we can check that font parameter. % \def\ifusingtt#1#2{\ifdim \fontdimen3\font=0pt #1\else #2\fi} % Same as above, but check for italic font. Actually this also catches % non-italic slanted fonts since it is impossible to distinguish them from % italic fonts. But since this is only used by $ and it uses \sl anyway % this is not a problem. \def\ifusingit#1#2{\ifdim \fontdimen1\font>0pt #1\else #2\fi} % Set catcodes for Texinfo file % Active characters for printing the wanted glyph. % Most of these we simply print from the \tt font, but for some, we can % use math or other variants that look better in normal text. % \catcode`\"=\active \def\activedoublequote{{\tt\char34}} \let"=\activedoublequote \catcode`\~=\active \def\activetilde{{\tt\char126}} \let~ = \activetilde \chardef\hatchar=`\^ \catcode`\^=\active \def\activehat{{\tt \hatchar}} \let^ = \activehat \catcode`\_=\active \def_{\ifusingtt\normalunderscore\_} \def\_{\leavevmode \kern.07em \vbox{\hrule width.3em height.1ex}\kern .07em } \let\realunder=_ \catcode`\|=\active \def|{{\tt\char124}} \chardef \less=`\< \catcode`\<=\active \def\activeless{{\tt \less}}\let< = \activeless \chardef \gtr=`\> \catcode`\>=\active \def\activegtr{{\tt \gtr}}\let> = \activegtr \catcode`\+=\active \def+{{\tt \char 43}} \catcode`\$=\active \def${\ifusingit{{\sl\$}}\normaldollar}%$ font-lock fix \catcode`\-=\active \let-=\normaldash % used for headline/footline in the output routine, in case the page % breaks in the middle of an @tex block. \def\texinfochars{% \let< = \activeless \let> = \activegtr \let~ = \activetilde \let^ = \activehat \markupsetuplqdefault \markupsetuprqdefault \let\b = \strong \let\i = \smartitalic % in principle, all other definitions in \tex have to be undone too. } % Used sometimes to turn off (effectively) the active characters even after % parsing them. \def\turnoffactive{% \normalturnoffactive \otherbackslash } \catcode`\@=0 % \backslashcurfont outputs one backslash character in current font, % as in \char`\\. \global\chardef\backslashcurfont=`\\ \global\let\rawbackslashxx=\backslashcurfont % let existing .??s files work % \realbackslash is an actual character `\' with catcode other, and % \doublebackslash is two of them (for the pdf outlines). {\catcode`\\=\other @gdef@realbackslash{\} @gdef@doublebackslash{\\}} % In Texinfo, backslash is an active character; it prints the backslash % in fixed width font. \catcode`\\=\active % @ for escape char from now on. % Print a typewriter backslash. For math mode, we can't simply use % \backslashcurfont: the story here is that in math mode, the \char % of \backslashcurfont ends up printing the roman \ from the math symbol % font (because \char in math mode uses the \mathcode, and plain.tex % sets \mathcode`\\="026E). Hence we use an explicit \mathchar, % which is the decimal equivalent of "715c (class 7, e.g., use \fam; % ignored family value; char position "5C). We can't use " for the % usual hex value because it has already been made active. @def@ttbackslash{{@tt @ifmmode @mathchar29020 @else @backslashcurfont @fi}} @let@backslashchar = @ttbackslash % @backslashchar{} is for user documents. % \rawbackslash defines an active \ to do \backslashcurfont. % \otherbackslash defines an active \ to be a literal `\' character with % catcode other. We switch back and forth between these. @gdef@rawbackslash{@let\=@backslashcurfont} @gdef@otherbackslash{@let\=@realbackslash} % Same as @turnoffactive except outputs \ as {\tt\char`\\} instead of % the literal character `\'. % {@catcode`- = @active @gdef@normalturnoffactive{% @passthroughcharstrue @let-=@normaldash @let"=@normaldoublequote @let$=@normaldollar %$ font-lock fix @let+=@normalplus @let<=@normalless @let>=@normalgreater @let^=@normalcaret @let_=@normalunderscore @let|=@normalverticalbar @let~=@normaltilde @let\=@ttbackslash @markupsetuplqdefault @markupsetuprqdefault @unsepspaces } } % If a .fmt file is being used, characters that might appear in a file % name cannot be active until we have parsed the command line. % So turn them off again, and have @fixbackslash turn them back on. @catcode`+=@other @catcode`@_=@other % \enablebackslashhack - allow file to begin `\input texinfo' % % If a .fmt file is being used, we don't want the `\input texinfo' to show up. % That is what \eatinput is for; after that, the `\' should revert to printing % a backslash. % If the file did not have a `\input texinfo', then it is turned off after % the first line; otherwise the first `\' in the file would cause an error. % This is used on the very last line of this file, texinfo.tex. % We also use @c to call @fixbackslash, in case ends of lines are hidden. { @catcode`@^=7 @catcode`@^^M=13@gdef@enablebackslashhack{% @global@let\ = @eatinput% @catcode`@^^M=13% @def@c{@fixbackslash@c}% % Definition for the newline at the end of this file. @def ^^M{@let^^M@secondlinenl}% % Definition for a newline in the main Texinfo file. @gdef @secondlinenl{@fixbackslash}% }} {@catcode`@^=7 @catcode`@^^M=13% @gdef@eatinput input texinfo#1^^M{@fixbackslash}} % Emergency active definition of newline, in case an active newline token % appears by mistake. {@catcode`@^=7 @catcode13=13% @gdef@enableemergencynewline{% @gdef^^M{% @par% %<warning: active newline>@par% }}} @gdef@fixbackslash{% @ifx\@eatinput @let\ = @ttbackslash @fi @catcode13=5 % regular end of line @enableemergencynewline @let@c=@texinfoc % Also turn back on active characters that might appear in the input % file name, in case not using a pre-dumped format. @catcode`+=@active @catcode`@_=@active % % If texinfo.cnf is present on the system, read it. % Useful for site-wide @afourpaper, etc. This macro, @fixbackslash, gets % called at the beginning of every Texinfo file. Not opening texinfo.cnf % directly in this file, texinfo.tex, makes it possible to make a format % file for Texinfo. % @openin 1 texinfo.cnf @ifeof 1 @else @input texinfo.cnf @fi @closein 1 } % Say @foo, not \foo, in error messages. @escapechar = `@@ % These (along with & and #) are made active for url-breaking, so need % active definitions as the normal characters. @def@normaldot{.} @def@normalquest{?} @def@normalslash{/} % These look ok in all fonts, so just make them not special. % @hashchar{} gets its own user-level command, because of #line. @catcode`@& = @other @def@normalamp{&} @catcode`@# = @other @def@normalhash{#} @catcode`@% = @other @def@normalpercent{%} @let @hashchar = @normalhash @c Finally, make ` and ' active, so that txicodequoteundirected and @c txicodequotebacktick work right in, e.g., @w{@code{`foo'}}. If we @c don't make ` and ' active, @code will not get them as active chars. @c Do this last of all since we use ` in the previous @catcode assignments. @catcode`@'=@active @catcode`@`=@active @markupsetuplqdefault @markupsetuprqdefault @c Local variables: @c eval: (add-hook 'write-file-hooks 'time-stamp) @c page-delimiter: "^\\\\message\\|emacs-page" @c time-stamp-start: "def\\\\texinfoversion{" @c time-stamp-format: "%:y-%02m-%02d.%02H" @c time-stamp-end: "}" @c End: @c vim:sw=2: @enablebackslashhack ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.2.33-8a3b/bootstrapped/build-aux/mdate-sh������������������������������������������������0000755�0001750�0001750�00000013640�12744162475�017165� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������#!/bin/sh # Get modification time of a file or directory and pretty-print it. scriptversion=2016-01-11.22; # UTC # Copyright (C) 1995-2015 Free Software Foundation, Inc. # written by Ulrich Drepper <drepper@gnu.ai.mit.edu>, June 1995 # # This program is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 2, or (at your option) # any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see <http://www.gnu.org/licenses/>. # As a special exception to the GNU General Public License, if you # distribute this file as part of a program that contains a # configuration script generated by Autoconf, you may include it under # the same distribution terms that you use for the rest of that program. # This file is maintained in Automake, please report # bugs to <bug-automake@gnu.org> or send patches to # <automake-patches@gnu.org>. if test -n "${ZSH_VERSION+set}" && (emulate sh) >/dev/null 2>&1; then emulate sh NULLCMD=: # Pre-4.2 versions of Zsh do word splitting on ${1+"$@"}, which # is contrary to our usage. Disable this feature. alias -g '${1+"$@"}'='"$@"' setopt NO_GLOB_SUBST fi case $1 in '') echo "$0: No file. Try '$0 --help' for more information." 1>&2 exit 1; ;; -h | --h*) cat <<\EOF Usage: mdate-sh [--help] [--version] FILE Pretty-print the modification day of FILE, in the format: 1 January 1970 Report bugs to <bug-automake@gnu.org>. EOF exit $? ;; -v | --v*) echo "mdate-sh $scriptversion" exit $? ;; esac error () { echo "$0: $1" >&2 exit 1 } # Prevent date giving response in another language. LANG=C export LANG LC_ALL=C export LC_ALL LC_TIME=C export LC_TIME # GNU ls changes its time format in response to the TIME_STYLE # variable. Since we cannot assume 'unset' works, revert this # variable to its documented default. if test "${TIME_STYLE+set}" = set; then TIME_STYLE=posix-long-iso export TIME_STYLE fi save_arg1=$1 # Find out how to get the extended ls output of a file or directory. if ls -L /dev/null 1>/dev/null 2>&1; then ls_command='ls -L -l -d' else ls_command='ls -l -d' fi # Avoid user/group names that might have spaces, when possible. if ls -n /dev/null 1>/dev/null 2>&1; then ls_command="$ls_command -n" fi # A 'ls -l' line looks as follows on OS/2. # drwxrwx--- 0 Aug 11 2001 foo # This differs from Unix, which adds ownership information. # drwxrwx--- 2 root root 4096 Aug 11 2001 foo # # To find the date, we split the line on spaces and iterate on words # until we find a month. This cannot work with files whose owner is a # user named "Jan", or "Feb", etc. However, it's unlikely that '/' # will be owned by a user whose name is a month. So we first look at # the extended ls output of the root directory to decide how many # words should be skipped to get the date. # On HPUX /bin/sh, "set" interprets "-rw-r--r--" as options, so the "x" below. set x`$ls_command /` # Find which argument is the month. month= command= until test $month do test $# -gt 0 || error "failed parsing '$ls_command /' output" shift # Add another shift to the command. command="$command shift;" case $1 in Jan) month=January; nummonth=1;; Feb) month=February; nummonth=2;; Mar) month=March; nummonth=3;; Apr) month=April; nummonth=4;; May) month=May; nummonth=5;; Jun) month=June; nummonth=6;; Jul) month=July; nummonth=7;; Aug) month=August; nummonth=8;; Sep) month=September; nummonth=9;; Oct) month=October; nummonth=10;; Nov) month=November; nummonth=11;; Dec) month=December; nummonth=12;; esac done test -n "$month" || error "failed parsing '$ls_command /' output" # Get the extended ls output of the file or directory. set dummy x`eval "$ls_command \"\\\$save_arg1\""` # Remove all preceding arguments eval $command # Because of the dummy argument above, month is in $2. # # On a POSIX system, we should have # # $# = 5 # $1 = file size # $2 = month # $3 = day # $4 = year or time # $5 = filename # # On Darwin 7.7.0 and 7.6.0, we have # # $# = 4 # $1 = day # $2 = month # $3 = year or time # $4 = filename # Get the month. case $2 in Jan) month=January; nummonth=1;; Feb) month=February; nummonth=2;; Mar) month=March; nummonth=3;; Apr) month=April; nummonth=4;; May) month=May; nummonth=5;; Jun) month=June; nummonth=6;; Jul) month=July; nummonth=7;; Aug) month=August; nummonth=8;; Sep) month=September; nummonth=9;; Oct) month=October; nummonth=10;; Nov) month=November; nummonth=11;; Dec) month=December; nummonth=12;; esac case $3 in ???*) day=$1;; *) day=$3; shift;; esac # Here we have to deal with the problem that the ls output gives either # the time of day or the year. case $3 in *:*) set `date`; eval year=\$$# case $2 in Jan) nummonthtod=1;; Feb) nummonthtod=2;; Mar) nummonthtod=3;; Apr) nummonthtod=4;; May) nummonthtod=5;; Jun) nummonthtod=6;; Jul) nummonthtod=7;; Aug) nummonthtod=8;; Sep) nummonthtod=9;; Oct) nummonthtod=10;; Nov) nummonthtod=11;; Dec) nummonthtod=12;; esac # For the first six month of the year the time notation can also # be used for files modified in the last year. if (expr $nummonth \> $nummonthtod) > /dev/null; then year=`expr $year - 1` fi;; *) year=$3;; esac # The result. echo $day $month $year # Local Variables: # mode: shell-script # sh-indentation: 2 # eval: (add-hook 'write-file-hooks 'time-stamp) # time-stamp-start: "scriptversion=" # time-stamp-format: "%:y-%02m-%02d.%02H" # time-stamp-time-zone: "UTC0" # time-stamp-end: "; # UTC" # End: ������������������������������������������������������������������������������������������������gnuastro-0.2.33-8a3b/bootstrapped/build-aux/depcomp�������������������������������������������������0000755�0001750�0001750�00000053701�12744162475�017114� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������#! /bin/sh # depcomp - compile a program generating dependencies as side-effects scriptversion=2016-01-11.22; # UTC # Copyright (C) 1999-2015 Free Software Foundation, Inc. # This program is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 2, or (at your option) # any later version. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # You should have received a copy of the GNU General Public License # along with this program. If not, see <http://www.gnu.org/licenses/>. # As a special exception to the GNU General Public License, if you # distribute this file as part of a program that contains a # configuration script generated by Autoconf, you may include it under # the same distribution terms that you use for the rest of that program. # Originally written by Alexandre Oliva <oliva@dcc.unicamp.br>. case $1 in '') echo "$0: No command. Try '$0 --help' for more information." 1>&2 exit 1; ;; -h | --h*) cat <<\EOF Usage: depcomp [--help] [--version] PROGRAM [ARGS] Run PROGRAMS ARGS to compile a file, generating dependencies as side-effects. Environment variables: depmode Dependency tracking mode. source Source file read by 'PROGRAMS ARGS'. object Object file output by 'PROGRAMS ARGS'. DEPDIR directory where to store dependencies. depfile Dependency file to output. tmpdepfile Temporary file to use when outputting dependencies. libtool Whether libtool is used (yes/no). Report bugs to <bug-automake@gnu.org>. EOF exit $? ;; -v | --v*) echo "depcomp $scriptversion" exit $? ;; esac # Get the directory component of the given path, and save it in the # global variables '$dir'. Note that this directory component will # be either empty or ending with a '/' character. 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We # parameterize here, but still list the modes in the big case below, # to make depend.m4 easier to write. Note that we *cannot* use a case # here, because this file can only contain one case statement. if test "$depmode" = hp; then # HP compiler uses -M and no extra arg. gccflag=-M depmode=gcc fi if test "$depmode" = dashXmstdout; then # This is just like dashmstdout with a different argument. dashmflag=-xM depmode=dashmstdout fi cygpath_u="cygpath -u -f -" if test "$depmode" = msvcmsys; then # This is just like msvisualcpp but w/o cygpath translation. # Just convert the backslash-escaped backslashes to single forward # slashes to satisfy depend.m4 cygpath_u='sed s,\\\\,/,g' depmode=msvisualcpp fi if test "$depmode" = msvc7msys; then # This is just like msvc7 but w/o cygpath translation. # Just convert the backslash-escaped backslashes to single forward # slashes to satisfy depend.m4 cygpath_u='sed s,\\\\,/,g' depmode=msvc7 fi if test "$depmode" = xlc; then # IBM C/C++ Compilers xlc/xlC can output gcc-like dependency information. gccflag=-qmakedep=gcc,-MF depmode=gcc fi case "$depmode" in gcc3) ## gcc 3 implements dependency tracking that does exactly what ## we want. Yay! Note: for some reason libtool 1.4 doesn't like ## it if -MD -MP comes after the -MF stuff. Hmm. ## Unfortunately, FreeBSD c89 acceptance of flags depends upon ## the command line argument order; so add the flags where they ## appear in depend2.am. Note that the slowdown incurred here ## affects only configure: in makefiles, %FASTDEP% shortcuts this. for arg do case $arg in -c) set fnord "$@" -MT "$object" -MD -MP -MF "$tmpdepfile" "$arg" ;; *) set fnord "$@" "$arg" ;; esac shift # fnord shift # $arg done "$@" stat=$? if test $stat -ne 0; then rm -f "$tmpdepfile" exit $stat fi mv "$tmpdepfile" "$depfile" ;; gcc) ## Note that this doesn't just cater to obsosete pre-3.x GCC compilers. ## but also to in-use compilers like IMB xlc/xlC and the HP C compiler. ## (see the conditional assignment to $gccflag above). ## There are various ways to get dependency output from gcc. Here's ## why we pick this rather obscure method: ## - Don't want to use -MD because we'd like the dependencies to end ## up in a subdir. Having to rename by hand is ugly. ## (We might end up doing this anyway to support other compilers.) ## - The DEPENDENCIES_OUTPUT environment variable makes gcc act like ## -MM, not -M (despite what the docs say). 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On the theory ## that the space means something, we add a space to the output as ## well. hp depmode also adds that space, but also prefixes the VPATH ## to the object. Take care to not repeat it in the output. ## Some versions of the HPUX 10.20 sed can't process this invocation ## correctly. Breaking it into two sed invocations is a workaround. tr ' ' "$nl" < "$tmpdepfile" \ | sed -e 's/^\\$//' -e '/^$/d' -e "s|.*$object$||" -e '/:$/d' \ | sed -e 's/$/ :/' >> "$depfile" rm -f "$tmpdepfile" ;; hp) # This case exists only to let depend.m4 do its work. It works by # looking at the text of this script. This case will never be run, # since it is checked for above. exit 1 ;; xlc) # This case exists only to let depend.m4 do its work. It works by # looking at the text of this script. This case will never be run, # since it is checked for above. exit 1 ;; aix) # The C for AIX Compiler uses -M and outputs the dependencies # in a .u file. 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"$@" -MD -MF "$tmpdepfile" stat=$? if test $stat -ne 0; then rm -f "$tmpdepfile" exit $stat fi rm -f "$depfile" # Each non-empty line is of the form 'foo.o : \' or ' dep.h \'. # We have to change lines of the first kind to '$object: \'. sed -e "s|.*:|$object :|" < "$tmpdepfile" > "$depfile" # And for each line of the second kind, we have to emit a 'dep.h:' # dummy dependency, to avoid the deleted-header problem. sed -n -e 's|^ *\(.*\) *\\$|\1:|p' < "$tmpdepfile" >> "$depfile" rm -f "$tmpdepfile" ;; ## The order of this option in the case statement is important, since the ## shell code in configure will try each of these formats in the order ## listed in this file. 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There is NO # warranty; not even for MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. # GNU Libtool is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 2 of the License, or # (at your option) any later version. # # As a special exception to the GNU General Public License, # if you distribute this file as part of a program or library that # is built using GNU Libtool, you may include this file under the # same distribution terms that you use for the rest of that program. # # GNU Libtool is distributed in the hope that it will be useful, but # WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU # General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see <http://www.gnu.org/licenses/>. PROGRAM=libtool PACKAGE=libtool VERSION=2.4.6 package_revision=2.4.6 ## ------ ## ## Usage. ## ## ------ ## # Run './libtool --help' for help with using this script from the # command line. ## ------------------------------- ## ## User overridable command paths. ## ## ------------------------------- ## # After configure completes, it has a better idea of some of the # shell tools we need than the defaults used by the functions shared # with bootstrap, so set those here where they can still be over- # ridden by the user, but otherwise take precedence. : ${AUTOCONF="autoconf"} : ${AUTOMAKE="automake"} ## -------------------------- ## ## Source external libraries. ## ## -------------------------- ## # Much of our low-level functionality needs to be sourced from external # libraries, which are installed to $pkgauxdir. # Set a version string for this script. scriptversion=2015-01-20.17; # UTC # General shell script boiler plate, and helper functions. # Written by Gary V. Vaughan, 2004 # Copyright (C) 2004-2015 Free Software Foundation, Inc. # This is free software; see the source for copying conditions. There is NO # warranty; not even for MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. # This program is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # As a special exception to the GNU General Public License, if you distribute # this file as part of a program or library that is built using GNU Libtool, # you may include this file under the same distribution terms that you use # for the rest of that program. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNES FOR A PARTICULAR PURPOSE. See the GNU # General Public License for more details. # You should have received a copy of the GNU General Public License # along with this program. If not, see <http://www.gnu.org/licenses/>. # Please report bugs or propose patches to gary@gnu.org. ## ------ ## ## Usage. ## ## ------ ## # Evaluate this file near the top of your script to gain access to # the functions and variables defined here: # # . `echo "$0" | ${SED-sed} 's|[^/]*$||'`/build-aux/funclib.sh # # If you need to override any of the default environment variable # settings, do that before evaluating this file. ## -------------------- ## ## Shell normalisation. ## ## -------------------- ## # Some shells need a little help to be as Bourne compatible as possible. # Before doing anything else, make sure all that help has been provided! DUALCASE=1; export DUALCASE # for MKS sh if test -n "${ZSH_VERSION+set}" && (emulate sh) >/dev/null 2>&1; then : emulate sh NULLCMD=: # Pre-4.2 versions of Zsh do word splitting on ${1+"$@"}, which # is contrary to our usage. Disable this feature. alias -g '${1+"$@"}'='"$@"' setopt NO_GLOB_SUBST else case `(set -o) 2>/dev/null` in *posix*) set -o posix ;; esac fi # NLS nuisances: We save the old values in case they are required later. _G_user_locale= _G_safe_locale= for _G_var in LANG LANGUAGE LC_ALL LC_CTYPE LC_COLLATE LC_MESSAGES do eval "if test set = \"\${$_G_var+set}\"; then save_$_G_var=\$$_G_var $_G_var=C export $_G_var _G_user_locale=\"$_G_var=\\\$save_\$_G_var; \$_G_user_locale\" _G_safe_locale=\"$_G_var=C; \$_G_safe_locale\" fi" done # CDPATH. (unset CDPATH) >/dev/null 2>&1 && unset CDPATH # Make sure IFS has a sensible default sp=' ' nl=' ' IFS="$sp $nl" # There are apparently some retarded systems that use ';' as a PATH separator! if test "${PATH_SEPARATOR+set}" != set; then PATH_SEPARATOR=: (PATH='/bin;/bin'; FPATH=$PATH; sh -c :) >/dev/null 2>&1 && { (PATH='/bin:/bin'; FPATH=$PATH; sh -c :) >/dev/null 2>&1 || PATH_SEPARATOR=';' } fi ## ------------------------- ## ## Locate command utilities. ## ## ------------------------- ## # func_executable_p FILE # ---------------------- # Check that FILE is an executable regular file. func_executable_p () { test -f "$1" && test -x "$1" } # func_path_progs PROGS_LIST CHECK_FUNC [PATH] # -------------------------------------------- # Search for either a program that responds to --version with output # containing "GNU", or else returned by CHECK_FUNC otherwise, by # trying all the directories in PATH with each of the elements of # PROGS_LIST. # # CHECK_FUNC should accept the path to a candidate program, and # set $func_check_prog_result if it truncates its output less than # $_G_path_prog_max characters. func_path_progs () { _G_progs_list=$1 _G_check_func=$2 _G_PATH=${3-"$PATH"} _G_path_prog_max=0 _G_path_prog_found=false _G_save_IFS=$IFS; IFS=${PATH_SEPARATOR-:} for _G_dir in $_G_PATH; do IFS=$_G_save_IFS test -z "$_G_dir" && _G_dir=. for _G_prog_name in $_G_progs_list; do for _exeext in '' .EXE; do _G_path_prog=$_G_dir/$_G_prog_name$_exeext func_executable_p "$_G_path_prog" || continue case `"$_G_path_prog" --version 2>&1` in *GNU*) func_path_progs_result=$_G_path_prog _G_path_prog_found=: ;; *) $_G_check_func $_G_path_prog func_path_progs_result=$func_check_prog_result ;; esac $_G_path_prog_found && break 3 done done done IFS=$_G_save_IFS test -z "$func_path_progs_result" && { echo "no acceptable sed could be found in \$PATH" >&2 exit 1 } } # We want to be able to use the functions in this file before configure # has figured out where the best binaries are kept, which means we have # to search for them ourselves - except when the results are already set # where we skip the searches. # Unless the user overrides by setting SED, search the path for either GNU # sed, or the sed that truncates its output the least. test -z "$SED" && { _G_sed_script=s/aaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaa/bbbbbbbbbbbbbbbbbbbbbbbbbbbbbbbbb/ for _G_i in 1 2 3 4 5 6 7; do _G_sed_script=$_G_sed_script$nl$_G_sed_script done echo "$_G_sed_script" 2>/dev/null | sed 99q >conftest.sed _G_sed_script= func_check_prog_sed () { _G_path_prog=$1 _G_count=0 printf 0123456789 >conftest.in while : do cat conftest.in conftest.in >conftest.tmp mv conftest.tmp conftest.in cp conftest.in conftest.nl echo '' >> conftest.nl "$_G_path_prog" -f conftest.sed <conftest.nl >conftest.out 2>/dev/null || break diff conftest.out conftest.nl >/dev/null 2>&1 || break _G_count=`expr $_G_count + 1` if test "$_G_count" -gt "$_G_path_prog_max"; then # Best one so far, save it but keep looking for a better one func_check_prog_result=$_G_path_prog _G_path_prog_max=$_G_count fi # 10*(2^10) chars as input seems more than enough test 10 -lt "$_G_count" && break done rm -f conftest.in conftest.tmp conftest.nl conftest.out } func_path_progs "sed gsed" func_check_prog_sed $PATH:/usr/xpg4/bin rm -f conftest.sed SED=$func_path_progs_result } # Unless the user overrides by setting GREP, search the path for either GNU # grep, or the grep that truncates its output the least. test -z "$GREP" && { func_check_prog_grep () { _G_path_prog=$1 _G_count=0 _G_path_prog_max=0 printf 0123456789 >conftest.in while : do cat conftest.in conftest.in >conftest.tmp mv conftest.tmp conftest.in cp conftest.in conftest.nl echo 'GREP' >> conftest.nl "$_G_path_prog" -e 'GREP$' -e '-(cannot match)-' <conftest.nl >conftest.out 2>/dev/null || break diff conftest.out conftest.nl >/dev/null 2>&1 || break _G_count=`expr $_G_count + 1` if test "$_G_count" -gt "$_G_path_prog_max"; then # Best one so far, save it but keep looking for a better one func_check_prog_result=$_G_path_prog _G_path_prog_max=$_G_count fi # 10*(2^10) chars as input seems more than enough test 10 -lt "$_G_count" && break done rm -f conftest.in conftest.tmp conftest.nl conftest.out } func_path_progs "grep ggrep" func_check_prog_grep $PATH:/usr/xpg4/bin GREP=$func_path_progs_result } ## ------------------------------- ## ## User overridable command paths. ## ## ------------------------------- ## # All uppercase variable names are used for environment variables. These # variables can be overridden by the user before calling a script that # uses them if a suitable command of that name is not already available # in the command search PATH. : ${CP="cp -f"} : ${ECHO="printf %s\n"} : ${EGREP="$GREP -E"} : ${FGREP="$GREP -F"} : ${LN_S="ln -s"} : ${MAKE="make"} : ${MKDIR="mkdir"} : ${MV="mv -f"} : ${RM="rm -f"} : ${SHELL="${CONFIG_SHELL-/bin/sh}"} ## -------------------- ## ## Useful sed snippets. ## ## -------------------- ## sed_dirname='s|/[^/]*$||' sed_basename='s|^.*/||' # Sed substitution that helps us do robust quoting. It backslashifies # metacharacters that are still active within double-quoted strings. sed_quote_subst='s|\([`"$\\]\)|\\\1|g' # Same as above, but do not quote variable references. sed_double_quote_subst='s/\(["`\\]\)/\\\1/g' # Sed substitution that turns a string into a regex matching for the # string literally. sed_make_literal_regex='s|[].[^$\\*\/]|\\&|g' # Sed substitution that converts a w32 file name or path # that contains forward slashes, into one that contains # (escaped) backslashes. A very naive implementation. sed_naive_backslashify='s|\\\\*|\\|g;s|/|\\|g;s|\\|\\\\|g' # Re-'\' parameter expansions in output of sed_double_quote_subst that # were '\'-ed in input to the same. If an odd number of '\' preceded a # '$' in input to sed_double_quote_subst, that '$' was protected from # expansion. Since each input '\' is now two '\'s, look for any number # of runs of four '\'s followed by two '\'s and then a '$'. '\' that '$'. _G_bs='\\' _G_bs2='\\\\' _G_bs4='\\\\\\\\' _G_dollar='\$' sed_double_backslash="\ s/$_G_bs4/&\\ /g s/^$_G_bs2$_G_dollar/$_G_bs&/ s/\\([^$_G_bs]\\)$_G_bs2$_G_dollar/\\1$_G_bs2$_G_bs$_G_dollar/g s/\n//g" ## ----------------- ## ## Global variables. ## ## ----------------- ## # Except for the global variables explicitly listed below, the following # functions in the '^func_' namespace, and the '^require_' namespace # variables initialised in the 'Resource management' section, sourcing # this file will not pollute your global namespace with anything # else. There's no portable way to scope variables in Bourne shell # though, so actually running these functions will sometimes place # results into a variable named after the function, and often use # temporary variables in the '^_G_' namespace. If you are careful to # avoid using those namespaces casually in your sourcing script, things # should continue to work as you expect. And, of course, you can freely # overwrite any of the functions or variables defined here before # calling anything to customize them. EXIT_SUCCESS=0 EXIT_FAILURE=1 EXIT_MISMATCH=63 # $? = 63 is used to indicate version mismatch to missing. EXIT_SKIP=77 # $? = 77 is used to indicate a skipped test to automake. # Allow overriding, eg assuming that you follow the convention of # putting '$debug_cmd' at the start of all your functions, you can get # bash to show function call trace with: # # debug_cmd='eval echo "${FUNCNAME[0]} $*" >&2' bash your-script-name debug_cmd=${debug_cmd-":"} exit_cmd=: # By convention, finish your script with: # # exit $exit_status # # so that you can set exit_status to non-zero if you want to indicate # something went wrong during execution without actually bailing out at # the point of failure. exit_status=$EXIT_SUCCESS # Work around backward compatibility issue on IRIX 6.5. On IRIX 6.4+, sh # is ksh but when the shell is invoked as "sh" and the current value of # the _XPG environment variable is not equal to 1 (one), the special # positional parameter $0, within a function call, is the name of the # function. progpath=$0 # The name of this program. progname=`$ECHO "$progpath" |$SED "$sed_basename"` # Make sure we have an absolute progpath for reexecution: case $progpath in [\\/]*|[A-Za-z]:\\*) ;; *[\\/]*) progdir=`$ECHO "$progpath" |$SED "$sed_dirname"` progdir=`cd "$progdir" && pwd` progpath=$progdir/$progname ;; *) _G_IFS=$IFS IFS=${PATH_SEPARATOR-:} for progdir in $PATH; do IFS=$_G_IFS test -x "$progdir/$progname" && break done IFS=$_G_IFS test -n "$progdir" || progdir=`pwd` progpath=$progdir/$progname ;; esac ## ----------------- ## ## Standard options. ## ## ----------------- ## # The following options affect the operation of the functions defined # below, and should be set appropriately depending on run-time para- # meters passed on the command line. opt_dry_run=false opt_quiet=false opt_verbose=false # Categories 'all' and 'none' are always available. Append any others # you will pass as the first argument to func_warning from your own # code. warning_categories= # By default, display warnings according to 'opt_warning_types'. Set # 'warning_func' to ':' to elide all warnings, or func_fatal_error to # treat the next displayed warning as a fatal error. warning_func=func_warn_and_continue # Set to 'all' to display all warnings, 'none' to suppress all # warnings, or a space delimited list of some subset of # 'warning_categories' to display only the listed warnings. opt_warning_types=all ## -------------------- ## ## Resource management. ## ## -------------------- ## # This section contains definitions for functions that each ensure a # particular resource (a file, or a non-empty configuration variable for # example) is available, and if appropriate to extract default values # from pertinent package files. Call them using their associated # 'require_*' variable to ensure that they are executed, at most, once. # # It's entirely deliberate that calling these functions can set # variables that don't obey the namespace limitations obeyed by the rest # of this file, in order that that they be as useful as possible to # callers. # require_term_colors # ------------------- # Allow display of bold text on terminals that support it. require_term_colors=func_require_term_colors func_require_term_colors () { $debug_cmd test -t 1 && { # COLORTERM and USE_ANSI_COLORS environment variables take # precedence, because most terminfo databases neglect to describe # whether color sequences are supported. test -n "${COLORTERM+set}" && : ${USE_ANSI_COLORS="1"} if test 1 = "$USE_ANSI_COLORS"; then # Standard ANSI escape sequences tc_reset='' tc_bold=''; tc_standout='' tc_red=''; tc_green='' tc_blue=''; tc_cyan='' else # Otherwise trust the terminfo database after all. test -n "`tput sgr0 2>/dev/null`" && { tc_reset=`tput sgr0` test -n "`tput bold 2>/dev/null`" && tc_bold=`tput bold` tc_standout=$tc_bold test -n "`tput smso 2>/dev/null`" && tc_standout=`tput smso` test -n "`tput setaf 1 2>/dev/null`" && tc_red=`tput setaf 1` test -n "`tput setaf 2 2>/dev/null`" && tc_green=`tput setaf 2` test -n "`tput setaf 4 2>/dev/null`" && tc_blue=`tput setaf 4` test -n "`tput setaf 5 2>/dev/null`" && tc_cyan=`tput setaf 5` } fi } require_term_colors=: } ## ----------------- ## ## Function library. ## ## ----------------- ## # This section contains a variety of useful functions to call in your # scripts. Take note of the portable wrappers for features provided by # some modern shells, which will fall back to slower equivalents on # less featureful shells. # func_append VAR VALUE # --------------------- # Append VALUE onto the existing contents of VAR. # We should try to minimise forks, especially on Windows where they are # unreasonably slow, so skip the feature probes when bash or zsh are # being used: if test set = "${BASH_VERSION+set}${ZSH_VERSION+set}"; then : ${_G_HAVE_ARITH_OP="yes"} : ${_G_HAVE_XSI_OPS="yes"} # The += operator was introduced in bash 3.1 case $BASH_VERSION in [12].* | 3.0 | 3.0*) ;; *) : ${_G_HAVE_PLUSEQ_OP="yes"} ;; esac fi # _G_HAVE_PLUSEQ_OP # Can be empty, in which case the shell is probed, "yes" if += is # useable or anything else if it does not work. test -z "$_G_HAVE_PLUSEQ_OP" \ && (eval 'x=a; x+=" b"; test "a b" = "$x"') 2>/dev/null \ && _G_HAVE_PLUSEQ_OP=yes if test yes = "$_G_HAVE_PLUSEQ_OP" then # This is an XSI compatible shell, allowing a faster implementation... eval 'func_append () { $debug_cmd eval "$1+=\$2" }' else # ...otherwise fall back to using expr, which is often a shell builtin. func_append () { $debug_cmd eval "$1=\$$1\$2" } fi # func_append_quoted VAR VALUE # ---------------------------- # Quote VALUE and append to the end of shell variable VAR, separated # by a space. if test yes = "$_G_HAVE_PLUSEQ_OP"; then eval 'func_append_quoted () { $debug_cmd func_quote_for_eval "$2" eval "$1+=\\ \$func_quote_for_eval_result" }' else func_append_quoted () { $debug_cmd func_quote_for_eval "$2" eval "$1=\$$1\\ \$func_quote_for_eval_result" } fi # func_append_uniq VAR VALUE # -------------------------- # Append unique VALUE onto the existing contents of VAR, assuming # entries are delimited by the first character of VALUE. For example: # # func_append_uniq options " --another-option option-argument" # # will only append to $options if " --another-option option-argument " # is not already present somewhere in $options already (note spaces at # each end implied by leading space in second argument). func_append_uniq () { $debug_cmd eval _G_current_value='`$ECHO $'$1'`' _G_delim=`expr "$2" : '\(.\)'` case $_G_delim$_G_current_value$_G_delim in *"$2$_G_delim"*) ;; *) func_append "$@" ;; esac } # func_arith TERM... # ------------------ # Set func_arith_result to the result of evaluating TERMs. test -z "$_G_HAVE_ARITH_OP" \ && (eval 'test 2 = $(( 1 + 1 ))') 2>/dev/null \ && _G_HAVE_ARITH_OP=yes if test yes = "$_G_HAVE_ARITH_OP"; then eval 'func_arith () { $debug_cmd func_arith_result=$(( $* )) }' else func_arith () { $debug_cmd func_arith_result=`expr "$@"` } fi # func_basename FILE # ------------------ # Set func_basename_result to FILE with everything up to and including # the last / stripped. if test yes = "$_G_HAVE_XSI_OPS"; then # If this shell supports suffix pattern removal, then use it to avoid # forking. Hide the definitions single quotes in case the shell chokes # on unsupported syntax... _b='func_basename_result=${1##*/}' _d='case $1 in */*) func_dirname_result=${1%/*}$2 ;; * ) func_dirname_result=$3 ;; esac' else # ...otherwise fall back to using sed. _b='func_basename_result=`$ECHO "$1" |$SED "$sed_basename"`' _d='func_dirname_result=`$ECHO "$1" |$SED "$sed_dirname"` if test "X$func_dirname_result" = "X$1"; then func_dirname_result=$3 else func_append func_dirname_result "$2" fi' fi eval 'func_basename () { $debug_cmd '"$_b"' }' # func_dirname FILE APPEND NONDIR_REPLACEMENT # ------------------------------------------- # Compute the dirname of FILE. If nonempty, add APPEND to the result, # otherwise set result to NONDIR_REPLACEMENT. eval 'func_dirname () { $debug_cmd '"$_d"' }' # func_dirname_and_basename FILE APPEND NONDIR_REPLACEMENT # -------------------------------------------------------- # Perform func_basename and func_dirname in a single function # call: # dirname: Compute the dirname of FILE. If nonempty, # add APPEND to the result, otherwise set result # to NONDIR_REPLACEMENT. # value returned in "$func_dirname_result" # basename: Compute filename of FILE. # value retuned in "$func_basename_result" # For efficiency, we do not delegate to the functions above but instead # duplicate the functionality here. eval 'func_dirname_and_basename () { $debug_cmd '"$_b"' '"$_d"' }' # func_echo ARG... # ---------------- # Echo program name prefixed message. func_echo () { $debug_cmd _G_message=$* func_echo_IFS=$IFS IFS=$nl for _G_line in $_G_message; do IFS=$func_echo_IFS $ECHO "$progname: $_G_line" done IFS=$func_echo_IFS } # func_echo_all ARG... # -------------------- # Invoke $ECHO with all args, space-separated. func_echo_all () { $ECHO "$*" } # func_echo_infix_1 INFIX ARG... # ------------------------------ # Echo program name, followed by INFIX on the first line, with any # additional lines not showing INFIX. func_echo_infix_1 () { $debug_cmd $require_term_colors _G_infix=$1; shift _G_indent=$_G_infix _G_prefix="$progname: $_G_infix: " _G_message=$* # Strip color escape sequences before counting printable length for _G_tc in "$tc_reset" "$tc_bold" "$tc_standout" "$tc_red" "$tc_green" "$tc_blue" "$tc_cyan" do test -n "$_G_tc" && { _G_esc_tc=`$ECHO "$_G_tc" | $SED "$sed_make_literal_regex"` _G_indent=`$ECHO "$_G_indent" | $SED "s|$_G_esc_tc||g"` } done _G_indent="$progname: "`echo "$_G_indent" | $SED 's|.| |g'`" " ## exclude from sc_prohibit_nested_quotes func_echo_infix_1_IFS=$IFS IFS=$nl for _G_line in $_G_message; do IFS=$func_echo_infix_1_IFS $ECHO "$_G_prefix$tc_bold$_G_line$tc_reset" >&2 _G_prefix=$_G_indent done IFS=$func_echo_infix_1_IFS } # func_error ARG... # ----------------- # Echo program name prefixed message to standard error. func_error () { $debug_cmd $require_term_colors func_echo_infix_1 " $tc_standout${tc_red}error$tc_reset" "$*" >&2 } # func_fatal_error ARG... # ----------------------- # Echo program name prefixed message to standard error, and exit. func_fatal_error () { $debug_cmd func_error "$*" exit $EXIT_FAILURE } # func_grep EXPRESSION FILENAME # ----------------------------- # Check whether EXPRESSION matches any line of FILENAME, without output. func_grep () { $debug_cmd $GREP "$1" "$2" >/dev/null 2>&1 } # func_len STRING # --------------- # Set func_len_result to the length of STRING. STRING may not # start with a hyphen. test -z "$_G_HAVE_XSI_OPS" \ && (eval 'x=a/b/c; test 5aa/bb/cc = "${#x}${x%%/*}${x%/*}${x#*/}${x##*/}"') 2>/dev/null \ && _G_HAVE_XSI_OPS=yes if test yes = "$_G_HAVE_XSI_OPS"; then eval 'func_len () { $debug_cmd func_len_result=${#1} }' else func_len () { $debug_cmd func_len_result=`expr "$1" : ".*" 2>/dev/null || echo $max_cmd_len` } fi # func_mkdir_p DIRECTORY-PATH # --------------------------- # Make sure the entire path to DIRECTORY-PATH is available. func_mkdir_p () { $debug_cmd _G_directory_path=$1 _G_dir_list= if test -n "$_G_directory_path" && test : != "$opt_dry_run"; then # Protect directory names starting with '-' case $_G_directory_path in -*) _G_directory_path=./$_G_directory_path ;; esac # While some portion of DIR does not yet exist... while test ! -d "$_G_directory_path"; do # ...make a list in topmost first order. Use a colon delimited # list incase some portion of path contains whitespace. _G_dir_list=$_G_directory_path:$_G_dir_list # If the last portion added has no slash in it, the list is done case $_G_directory_path in */*) ;; *) break ;; esac # ...otherwise throw away the child directory and loop _G_directory_path=`$ECHO "$_G_directory_path" | $SED -e "$sed_dirname"` done _G_dir_list=`$ECHO "$_G_dir_list" | $SED 's|:*$||'` func_mkdir_p_IFS=$IFS; IFS=: for _G_dir in $_G_dir_list; do IFS=$func_mkdir_p_IFS # mkdir can fail with a 'File exist' error if two processes # try to create one of the directories concurrently. Don't # stop in that case! $MKDIR "$_G_dir" 2>/dev/null || : done IFS=$func_mkdir_p_IFS # Bail out if we (or some other process) failed to create a directory. test -d "$_G_directory_path" || \ func_fatal_error "Failed to create '$1'" fi } # func_mktempdir [BASENAME] # ------------------------- # Make a temporary directory that won't clash with other running # libtool processes, and avoids race conditions if possible. If # given, BASENAME is the basename for that directory. func_mktempdir () { $debug_cmd _G_template=${TMPDIR-/tmp}/${1-$progname} if test : = "$opt_dry_run"; then # Return a directory name, but don't create it in dry-run mode _G_tmpdir=$_G_template-$$ else # If mktemp works, use that first and foremost _G_tmpdir=`mktemp -d "$_G_template-XXXXXXXX" 2>/dev/null` if test ! -d "$_G_tmpdir"; then # Failing that, at least try and use $RANDOM to avoid a race _G_tmpdir=$_G_template-${RANDOM-0}$$ func_mktempdir_umask=`umask` umask 0077 $MKDIR "$_G_tmpdir" umask $func_mktempdir_umask fi # If we're not in dry-run mode, bomb out on failure test -d "$_G_tmpdir" || \ func_fatal_error "cannot create temporary directory '$_G_tmpdir'" fi $ECHO "$_G_tmpdir" } # func_normal_abspath PATH # ------------------------ # Remove doubled-up and trailing slashes, "." path components, # and cancel out any ".." path components in PATH after making # it an absolute path. func_normal_abspath () { $debug_cmd # These SED scripts presuppose an absolute path with a trailing slash. _G_pathcar='s|^/\([^/]*\).*$|\1|' _G_pathcdr='s|^/[^/]*||' _G_removedotparts=':dotsl s|/\./|/|g t dotsl s|/\.$|/|' _G_collapseslashes='s|/\{1,\}|/|g' _G_finalslash='s|/*$|/|' # Start from root dir and reassemble the path. func_normal_abspath_result= func_normal_abspath_tpath=$1 func_normal_abspath_altnamespace= case $func_normal_abspath_tpath in "") # Empty path, that just means $cwd. func_stripname '' '/' "`pwd`" func_normal_abspath_result=$func_stripname_result return ;; # The next three entries are used to spot a run of precisely # two leading slashes without using negated character classes; # we take advantage of case's first-match behaviour. ///*) # Unusual form of absolute path, do nothing. ;; //*) # Not necessarily an ordinary path; POSIX reserves leading '//' # and for example Cygwin uses it to access remote file shares # over CIFS/SMB, so we conserve a leading double slash if found. func_normal_abspath_altnamespace=/ ;; /*) # Absolute path, do nothing. ;; *) # Relative path, prepend $cwd. func_normal_abspath_tpath=`pwd`/$func_normal_abspath_tpath ;; esac # Cancel out all the simple stuff to save iterations. We also want # the path to end with a slash for ease of parsing, so make sure # there is one (and only one) here. func_normal_abspath_tpath=`$ECHO "$func_normal_abspath_tpath" | $SED \ -e "$_G_removedotparts" -e "$_G_collapseslashes" -e "$_G_finalslash"` while :; do # Processed it all yet? if test / = "$func_normal_abspath_tpath"; then # If we ascended to the root using ".." the result may be empty now. if test -z "$func_normal_abspath_result"; then func_normal_abspath_result=/ fi break fi func_normal_abspath_tcomponent=`$ECHO "$func_normal_abspath_tpath" | $SED \ -e "$_G_pathcar"` func_normal_abspath_tpath=`$ECHO "$func_normal_abspath_tpath" | $SED \ -e "$_G_pathcdr"` # Figure out what to do with it case $func_normal_abspath_tcomponent in "") # Trailing empty path component, ignore it. ;; ..) # Parent dir; strip last assembled component from result. func_dirname "$func_normal_abspath_result" func_normal_abspath_result=$func_dirname_result ;; *) # Actual path component, append it. func_append func_normal_abspath_result "/$func_normal_abspath_tcomponent" ;; esac done # Restore leading double-slash if one was found on entry. func_normal_abspath_result=$func_normal_abspath_altnamespace$func_normal_abspath_result } # func_notquiet ARG... # -------------------- # Echo program name prefixed message only when not in quiet mode. func_notquiet () { $debug_cmd $opt_quiet || func_echo ${1+"$@"} # A bug in bash halts the script if the last line of a function # fails when set -e is in force, so we need another command to # work around that: : } # func_relative_path SRCDIR DSTDIR # -------------------------------- # Set func_relative_path_result to the relative path from SRCDIR to DSTDIR. func_relative_path () { $debug_cmd func_relative_path_result= func_normal_abspath "$1" func_relative_path_tlibdir=$func_normal_abspath_result func_normal_abspath "$2" func_relative_path_tbindir=$func_normal_abspath_result # Ascend the tree starting from libdir while :; do # check if we have found a prefix of bindir case $func_relative_path_tbindir in $func_relative_path_tlibdir) # found an exact match func_relative_path_tcancelled= break ;; $func_relative_path_tlibdir*) # found a matching prefix func_stripname "$func_relative_path_tlibdir" '' "$func_relative_path_tbindir" func_relative_path_tcancelled=$func_stripname_result if test -z "$func_relative_path_result"; then func_relative_path_result=. fi break ;; *) func_dirname $func_relative_path_tlibdir func_relative_path_tlibdir=$func_dirname_result if test -z "$func_relative_path_tlibdir"; then # Have to descend all the way to the root! func_relative_path_result=../$func_relative_path_result func_relative_path_tcancelled=$func_relative_path_tbindir break fi func_relative_path_result=../$func_relative_path_result ;; esac done # Now calculate path; take care to avoid doubling-up slashes. func_stripname '' '/' "$func_relative_path_result" func_relative_path_result=$func_stripname_result func_stripname '/' '/' "$func_relative_path_tcancelled" if test -n "$func_stripname_result"; then func_append func_relative_path_result "/$func_stripname_result" fi # Normalisation. If bindir is libdir, return '.' else relative path. if test -n "$func_relative_path_result"; then func_stripname './' '' "$func_relative_path_result" func_relative_path_result=$func_stripname_result fi test -n "$func_relative_path_result" || func_relative_path_result=. : } # func_quote_for_eval ARG... # -------------------------- # Aesthetically quote ARGs to be evaled later. # This function returns two values: # i) func_quote_for_eval_result # double-quoted, suitable for a subsequent eval # ii) func_quote_for_eval_unquoted_result # has all characters that are still active within double # quotes backslashified. func_quote_for_eval () { $debug_cmd func_quote_for_eval_unquoted_result= func_quote_for_eval_result= while test 0 -lt $#; do case $1 in *[\\\`\"\$]*) _G_unquoted_arg=`printf '%s\n' "$1" |$SED "$sed_quote_subst"` ;; *) _G_unquoted_arg=$1 ;; esac if test -n "$func_quote_for_eval_unquoted_result"; then func_append func_quote_for_eval_unquoted_result " $_G_unquoted_arg" else func_append func_quote_for_eval_unquoted_result "$_G_unquoted_arg" fi case $_G_unquoted_arg in # Double-quote args containing shell metacharacters to delay # word splitting, command substitution and variable expansion # for a subsequent eval. # Many Bourne shells cannot handle close brackets correctly # in scan sets, so we specify it separately. *[\[\~\#\^\&\*\(\)\{\}\|\;\<\>\?\'\ \ ]*|*]*|"") _G_quoted_arg=\"$_G_unquoted_arg\" ;; *) _G_quoted_arg=$_G_unquoted_arg ;; esac if test -n "$func_quote_for_eval_result"; then func_append func_quote_for_eval_result " $_G_quoted_arg" else func_append func_quote_for_eval_result "$_G_quoted_arg" fi shift done } # func_quote_for_expand ARG # ------------------------- # Aesthetically quote ARG to be evaled later; same as above, # but do not quote variable references. func_quote_for_expand () { $debug_cmd case $1 in *[\\\`\"]*) _G_arg=`$ECHO "$1" | $SED \ -e "$sed_double_quote_subst" -e "$sed_double_backslash"` ;; *) _G_arg=$1 ;; esac case $_G_arg in # Double-quote args containing shell metacharacters to delay # word splitting and command substitution for a subsequent eval. # Many Bourne shells cannot handle close brackets correctly # in scan sets, so we specify it separately. *[\[\~\#\^\&\*\(\)\{\}\|\;\<\>\?\'\ \ ]*|*]*|"") _G_arg=\"$_G_arg\" ;; esac func_quote_for_expand_result=$_G_arg } # func_stripname PREFIX SUFFIX NAME # --------------------------------- # strip PREFIX and SUFFIX from NAME, and store in func_stripname_result. # PREFIX and SUFFIX must not contain globbing or regex special # characters, hashes, percent signs, but SUFFIX may contain a leading # dot (in which case that matches only a dot). if test yes = "$_G_HAVE_XSI_OPS"; then eval 'func_stripname () { $debug_cmd # pdksh 5.2.14 does not do ${X%$Y} correctly if both X and Y are # positional parameters, so assign one to ordinary variable first. func_stripname_result=$3 func_stripname_result=${func_stripname_result#"$1"} func_stripname_result=${func_stripname_result%"$2"} }' else func_stripname () { $debug_cmd case $2 in .*) func_stripname_result=`$ECHO "$3" | $SED -e "s%^$1%%" -e "s%\\\\$2\$%%"`;; *) func_stripname_result=`$ECHO "$3" | $SED -e "s%^$1%%" -e "s%$2\$%%"`;; esac } fi # func_show_eval CMD [FAIL_EXP] # ----------------------------- # Unless opt_quiet is true, then output CMD. Then, if opt_dryrun is # not true, evaluate CMD. If the evaluation of CMD fails, and FAIL_EXP # is given, then evaluate it. func_show_eval () { $debug_cmd _G_cmd=$1 _G_fail_exp=${2-':'} func_quote_for_expand "$_G_cmd" eval "func_notquiet $func_quote_for_expand_result" $opt_dry_run || { eval "$_G_cmd" _G_status=$? if test 0 -ne "$_G_status"; then eval "(exit $_G_status); $_G_fail_exp" fi } } # func_show_eval_locale CMD [FAIL_EXP] # ------------------------------------ # Unless opt_quiet is true, then output CMD. Then, if opt_dryrun is # not true, evaluate CMD. If the evaluation of CMD fails, and FAIL_EXP # is given, then evaluate it. Use the saved locale for evaluation. func_show_eval_locale () { $debug_cmd _G_cmd=$1 _G_fail_exp=${2-':'} $opt_quiet || { func_quote_for_expand "$_G_cmd" eval "func_echo $func_quote_for_expand_result" } $opt_dry_run || { eval "$_G_user_locale $_G_cmd" _G_status=$? eval "$_G_safe_locale" if test 0 -ne "$_G_status"; then eval "(exit $_G_status); $_G_fail_exp" fi } } # func_tr_sh # ---------- # Turn $1 into a string suitable for a shell variable name. # Result is stored in $func_tr_sh_result. All characters # not in the set a-zA-Z0-9_ are replaced with '_'. Further, # if $1 begins with a digit, a '_' is prepended as well. func_tr_sh () { $debug_cmd case $1 in [0-9]* | *[!a-zA-Z0-9_]*) func_tr_sh_result=`$ECHO "$1" | $SED -e 's/^\([0-9]\)/_\1/' -e 's/[^a-zA-Z0-9_]/_/g'` ;; * ) func_tr_sh_result=$1 ;; esac } # func_verbose ARG... # ------------------- # Echo program name prefixed message in verbose mode only. func_verbose () { $debug_cmd $opt_verbose && func_echo "$*" : } # func_warn_and_continue ARG... # ----------------------------- # Echo program name prefixed warning message to standard error. func_warn_and_continue () { $debug_cmd $require_term_colors func_echo_infix_1 "${tc_red}warning$tc_reset" "$*" >&2 } # func_warning CATEGORY ARG... # ---------------------------- # Echo program name prefixed warning message to standard error. Warning # messages can be filtered according to CATEGORY, where this function # elides messages where CATEGORY is not listed in the global variable # 'opt_warning_types'. func_warning () { $debug_cmd # CATEGORY must be in the warning_categories list! case " $warning_categories " in *" $1 "*) ;; *) func_internal_error "invalid warning category '$1'" ;; esac _G_category=$1 shift case " $opt_warning_types " in *" $_G_category "*) $warning_func ${1+"$@"} ;; esac } # func_sort_ver VER1 VER2 # ----------------------- # 'sort -V' is not generally available. # Note this deviates from the version comparison in automake # in that it treats 1.5 < 1.5.0, and treats 1.4.4a < 1.4-p3a # but this should suffice as we won't be specifying old # version formats or redundant trailing .0 in bootstrap.conf. # If we did want full compatibility then we should probably # use m4_version_compare from autoconf. func_sort_ver () { $debug_cmd printf '%s\n%s\n' "$1" "$2" \ | sort -t. -k 1,1n -k 2,2n -k 3,3n -k 4,4n -k 5,5n -k 6,6n -k 7,7n -k 8,8n -k 9,9n } # func_lt_ver PREV CURR # --------------------- # Return true if PREV and CURR are in the correct order according to # func_sort_ver, otherwise false. Use it like this: # # func_lt_ver "$prev_ver" "$proposed_ver" || func_fatal_error "..." func_lt_ver () { $debug_cmd test "x$1" = x`func_sort_ver "$1" "$2" | $SED 1q` } # Local variables: # mode: shell-script # sh-indentation: 2 # eval: (add-hook 'before-save-hook 'time-stamp) # time-stamp-pattern: "10/scriptversion=%:y-%02m-%02d.%02H; # UTC" # time-stamp-time-zone: "UTC" # End: #! /bin/sh # Set a version string for this script. scriptversion=2014-01-07.03; # UTC # A portable, pluggable option parser for Bourne shell. # Written by Gary V. Vaughan, 2010 # Copyright (C) 2010-2015 Free Software Foundation, Inc. # This is free software; see the source for copying conditions. There is NO # warranty; not even for MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. # This program is free software: you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation, either version 3 of the License, or # (at your option) any later version. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # You should have received a copy of the GNU General Public License # along with this program. If not, see <http://www.gnu.org/licenses/>. # Please report bugs or propose patches to gary@gnu.org. ## ------ ## ## Usage. ## ## ------ ## # This file is a library for parsing options in your shell scripts along # with assorted other useful supporting features that you can make use # of too. # # For the simplest scripts you might need only: # # #!/bin/sh # . relative/path/to/funclib.sh # . relative/path/to/options-parser # scriptversion=1.0 # func_options ${1+"$@"} # eval set dummy "$func_options_result"; shift # ...rest of your script... # # In order for the '--version' option to work, you will need to have a # suitably formatted comment like the one at the top of this file # starting with '# Written by ' and ending with '# warranty; '. # # For '-h' and '--help' to work, you will also need a one line # description of your script's purpose in a comment directly above the # '# Written by ' line, like the one at the top of this file. # # The default options also support '--debug', which will turn on shell # execution tracing (see the comment above debug_cmd below for another # use), and '--verbose' and the func_verbose function to allow your script # to display verbose messages only when your user has specified # '--verbose'. # # After sourcing this file, you can plug processing for additional # options by amending the variables from the 'Configuration' section # below, and following the instructions in the 'Option parsing' # section further down. ## -------------- ## ## Configuration. ## ## -------------- ## # You should override these variables in your script after sourcing this # file so that they reflect the customisations you have added to the # option parser. # The usage line for option parsing errors and the start of '-h' and # '--help' output messages. You can embed shell variables for delayed # expansion at the time the message is displayed, but you will need to # quote other shell meta-characters carefully to prevent them being # expanded when the contents are evaled. usage='$progpath [OPTION]...' # Short help message in response to '-h' and '--help'. Add to this or # override it after sourcing this library to reflect the full set of # options your script accepts. usage_message="\ --debug enable verbose shell tracing -W, --warnings=CATEGORY report the warnings falling in CATEGORY [all] -v, --verbose verbosely report processing --version print version information and exit -h, --help print short or long help message and exit " # Additional text appended to 'usage_message' in response to '--help'. long_help_message=" Warning categories include: 'all' show all warnings 'none' turn off all the warnings 'error' warnings are treated as fatal errors" # Help message printed before fatal option parsing errors. fatal_help="Try '\$progname --help' for more information." ## ------------------------- ## ## Hook function management. ## ## ------------------------- ## # This section contains functions for adding, removing, and running hooks # to the main code. A hook is just a named list of of function, that can # be run in order later on. # func_hookable FUNC_NAME # ----------------------- # Declare that FUNC_NAME will run hooks added with # 'func_add_hook FUNC_NAME ...'. func_hookable () { $debug_cmd func_append hookable_fns " $1" } # func_add_hook FUNC_NAME HOOK_FUNC # --------------------------------- # Request that FUNC_NAME call HOOK_FUNC before it returns. FUNC_NAME must # first have been declared "hookable" by a call to 'func_hookable'. func_add_hook () { $debug_cmd case " $hookable_fns " in *" $1 "*) ;; *) func_fatal_error "'$1' does not accept hook functions." ;; esac eval func_append ${1}_hooks '" $2"' } # func_remove_hook FUNC_NAME HOOK_FUNC # ------------------------------------ # Remove HOOK_FUNC from the list of functions called by FUNC_NAME. func_remove_hook () { $debug_cmd eval ${1}_hooks='`$ECHO "\$'$1'_hooks" |$SED "s| '$2'||"`' } # func_run_hooks FUNC_NAME [ARG]... # --------------------------------- # Run all hook functions registered to FUNC_NAME. # It is assumed that the list of hook functions contains nothing more # than a whitespace-delimited list of legal shell function names, and # no effort is wasted trying to catch shell meta-characters or preserve # whitespace. func_run_hooks () { $debug_cmd case " $hookable_fns " in *" $1 "*) ;; *) func_fatal_error "'$1' does not support hook funcions.n" ;; esac eval _G_hook_fns=\$$1_hooks; shift for _G_hook in $_G_hook_fns; do eval $_G_hook '"$@"' # store returned options list back into positional # parameters for next 'cmd' execution. eval _G_hook_result=\$${_G_hook}_result eval set dummy "$_G_hook_result"; shift done func_quote_for_eval ${1+"$@"} func_run_hooks_result=$func_quote_for_eval_result } ## --------------- ## ## Option parsing. ## ## --------------- ## # In order to add your own option parsing hooks, you must accept the # full positional parameter list in your hook function, remove any # options that you action, and then pass back the remaining unprocessed # options in '<hooked_function_name>_result', escaped suitably for # 'eval'. Like this: # # my_options_prep () # { # $debug_cmd # # # Extend the existing usage message. # usage_message=$usage_message' # -s, --silent don'\''t print informational messages # ' # # func_quote_for_eval ${1+"$@"} # my_options_prep_result=$func_quote_for_eval_result # } # func_add_hook func_options_prep my_options_prep # # # my_silent_option () # { # $debug_cmd # # # Note that for efficiency, we parse as many options as we can # # recognise in a loop before passing the remainder back to the # # caller on the first unrecognised argument we encounter. # while test $# -gt 0; do # opt=$1; shift # case $opt in # --silent|-s) opt_silent=: ;; # # Separate non-argument short options: # -s*) func_split_short_opt "$_G_opt" # set dummy "$func_split_short_opt_name" \ # "-$func_split_short_opt_arg" ${1+"$@"} # shift # ;; # *) set dummy "$_G_opt" "$*"; shift; break ;; # esac # done # # func_quote_for_eval ${1+"$@"} # my_silent_option_result=$func_quote_for_eval_result # } # func_add_hook func_parse_options my_silent_option # # # my_option_validation () # { # $debug_cmd # # $opt_silent && $opt_verbose && func_fatal_help "\ # '--silent' and '--verbose' options are mutually exclusive." # # func_quote_for_eval ${1+"$@"} # my_option_validation_result=$func_quote_for_eval_result # } # func_add_hook func_validate_options my_option_validation # # You'll alse need to manually amend $usage_message to reflect the extra # options you parse. It's preferable to append if you can, so that # multiple option parsing hooks can be added safely. # func_options [ARG]... # --------------------- # All the functions called inside func_options are hookable. See the # individual implementations for details. func_hookable func_options func_options () { $debug_cmd func_options_prep ${1+"$@"} eval func_parse_options \ ${func_options_prep_result+"$func_options_prep_result"} eval func_validate_options \ ${func_parse_options_result+"$func_parse_options_result"} eval func_run_hooks func_options \ ${func_validate_options_result+"$func_validate_options_result"} # save modified positional parameters for caller func_options_result=$func_run_hooks_result } # func_options_prep [ARG]... # -------------------------- # All initialisations required before starting the option parse loop. # Note that when calling hook functions, we pass through the list of # positional parameters. If a hook function modifies that list, and # needs to propogate that back to rest of this script, then the complete # modified list must be put in 'func_run_hooks_result' before # returning. func_hookable func_options_prep func_options_prep () { $debug_cmd # Option defaults: opt_verbose=false opt_warning_types= func_run_hooks func_options_prep ${1+"$@"} # save modified positional parameters for caller func_options_prep_result=$func_run_hooks_result } # func_parse_options [ARG]... # --------------------------- # The main option parsing loop. func_hookable func_parse_options func_parse_options () { $debug_cmd func_parse_options_result= # this just eases exit handling while test $# -gt 0; do # Defer to hook functions for initial option parsing, so they # get priority in the event of reusing an option name. func_run_hooks func_parse_options ${1+"$@"} # Adjust func_parse_options positional parameters to match eval set dummy "$func_run_hooks_result"; shift # Break out of the loop if we already parsed every option. test $# -gt 0 || break _G_opt=$1 shift case $_G_opt in --debug|-x) debug_cmd='set -x' func_echo "enabling shell trace mode" $debug_cmd ;; --no-warnings|--no-warning|--no-warn) set dummy --warnings none ${1+"$@"} shift ;; --warnings|--warning|-W) test $# = 0 && func_missing_arg $_G_opt && break case " $warning_categories $1" in *" $1 "*) # trailing space prevents matching last $1 above func_append_uniq opt_warning_types " $1" ;; *all) opt_warning_types=$warning_categories ;; *none) opt_warning_types=none warning_func=: ;; *error) opt_warning_types=$warning_categories warning_func=func_fatal_error ;; *) func_fatal_error \ "unsupported warning category: '$1'" ;; esac shift ;; --verbose|-v) opt_verbose=: ;; --version) func_version ;; -\?|-h) func_usage ;; --help) func_help ;; # Separate optargs to long options (plugins may need this): --*=*) func_split_equals "$_G_opt" set dummy "$func_split_equals_lhs" \ "$func_split_equals_rhs" ${1+"$@"} shift ;; # Separate optargs to short options: -W*) func_split_short_opt "$_G_opt" set dummy "$func_split_short_opt_name" \ "$func_split_short_opt_arg" ${1+"$@"} shift ;; # Separate non-argument short options: -\?*|-h*|-v*|-x*) func_split_short_opt "$_G_opt" set dummy "$func_split_short_opt_name" \ "-$func_split_short_opt_arg" ${1+"$@"} shift ;; --) break ;; -*) func_fatal_help "unrecognised option: '$_G_opt'" ;; *) set dummy "$_G_opt" ${1+"$@"}; shift; break ;; esac done # save modified positional parameters for caller func_quote_for_eval ${1+"$@"} func_parse_options_result=$func_quote_for_eval_result } # func_validate_options [ARG]... # ------------------------------ # Perform any sanity checks on option settings and/or unconsumed # arguments. func_hookable func_validate_options func_validate_options () { $debug_cmd # Display all warnings if -W was not given. test -n "$opt_warning_types" || opt_warning_types=" $warning_categories" func_run_hooks func_validate_options ${1+"$@"} # Bail if the options were screwed! $exit_cmd $EXIT_FAILURE # save modified positional parameters for caller func_validate_options_result=$func_run_hooks_result } ## ----------------- ## ## Helper functions. ## ## ----------------- ## # This section contains the helper functions used by the rest of the # hookable option parser framework in ascii-betical order. # func_fatal_help ARG... # ---------------------- # Echo program name prefixed message to standard error, followed by # a help hint, and exit. func_fatal_help () { $debug_cmd eval \$ECHO \""Usage: $usage"\" eval \$ECHO \""$fatal_help"\" func_error ${1+"$@"} exit $EXIT_FAILURE } # func_help # --------- # Echo long help message to standard output and exit. func_help () { $debug_cmd func_usage_message $ECHO "$long_help_message" exit 0 } # func_missing_arg ARGNAME # ------------------------ # Echo program name prefixed message to standard error and set global # exit_cmd. func_missing_arg () { $debug_cmd func_error "Missing argument for '$1'." exit_cmd=exit } # func_split_equals STRING # ------------------------ # Set func_split_equals_lhs and func_split_equals_rhs shell variables after # splitting STRING at the '=' sign. test -z "$_G_HAVE_XSI_OPS" \ && (eval 'x=a/b/c; test 5aa/bb/cc = "${#x}${x%%/*}${x%/*}${x#*/}${x##*/}"') 2>/dev/null \ && _G_HAVE_XSI_OPS=yes if test yes = "$_G_HAVE_XSI_OPS" then # This is an XSI compatible shell, allowing a faster implementation... eval 'func_split_equals () { $debug_cmd func_split_equals_lhs=${1%%=*} func_split_equals_rhs=${1#*=} test "x$func_split_equals_lhs" = "x$1" \ && func_split_equals_rhs= }' else # ...otherwise fall back to using expr, which is often a shell builtin. func_split_equals () { $debug_cmd func_split_equals_lhs=`expr "x$1" : 'x\([^=]*\)'` func_split_equals_rhs= test "x$func_split_equals_lhs" = "x$1" \ || func_split_equals_rhs=`expr "x$1" : 'x[^=]*=\(.*\)$'` } fi #func_split_equals # func_split_short_opt SHORTOPT # ----------------------------- # Set func_split_short_opt_name and func_split_short_opt_arg shell # variables after splitting SHORTOPT after the 2nd character. if test yes = "$_G_HAVE_XSI_OPS" then # This is an XSI compatible shell, allowing a faster implementation... eval 'func_split_short_opt () { $debug_cmd func_split_short_opt_arg=${1#??} func_split_short_opt_name=${1%"$func_split_short_opt_arg"} }' else # ...otherwise fall back to using expr, which is often a shell builtin. func_split_short_opt () { $debug_cmd func_split_short_opt_name=`expr "x$1" : 'x-\(.\)'` func_split_short_opt_arg=`expr "x$1" : 'x-.\(.*\)$'` } fi #func_split_short_opt # func_usage # ---------- # Echo short help message to standard output and exit. func_usage () { $debug_cmd func_usage_message $ECHO "Run '$progname --help |${PAGER-more}' for full usage" exit 0 } # func_usage_message # ------------------ # Echo short help message to standard output. func_usage_message () { $debug_cmd eval \$ECHO \""Usage: $usage"\" echo $SED -n 's|^# || /^Written by/{ x;p;x } h /^Written by/q' < "$progpath" echo eval \$ECHO \""$usage_message"\" } # func_version # ------------ # Echo version message to standard output and exit. func_version () { $debug_cmd printf '%s\n' "$progname $scriptversion" $SED -n ' /(C)/!b go :more /\./!{ N s|\n# | | b more } :go /^# Written by /,/# warranty; / { s|^# || s|^# *$|| s|\((C)\)[ 0-9,-]*[ ,-]\([1-9][0-9]* \)|\1 \2| p } /^# Written by / { s|^# || p } /^warranty; /q' < "$progpath" exit $? } # Local variables: # mode: shell-script # sh-indentation: 2 # eval: (add-hook 'before-save-hook 'time-stamp) # time-stamp-pattern: "10/scriptversion=%:y-%02m-%02d.%02H; # UTC" # time-stamp-time-zone: "UTC" # End: # Set a version string. scriptversion='(GNU libtool) 2.4.6' # func_echo ARG... # ---------------- # Libtool also displays the current mode in messages, so override # funclib.sh func_echo with this custom definition. func_echo () { $debug_cmd _G_message=$* func_echo_IFS=$IFS IFS=$nl for _G_line in $_G_message; do IFS=$func_echo_IFS $ECHO "$progname${opt_mode+: $opt_mode}: $_G_line" done IFS=$func_echo_IFS } # func_warning ARG... # ------------------- # Libtool warnings are not categorized, so override funclib.sh # func_warning with this simpler definition. func_warning () { $debug_cmd $warning_func ${1+"$@"} } ## ---------------- ## ## Options parsing. ## ## ---------------- ## # Hook in the functions to make sure our own options are parsed during # the option parsing loop. usage='$progpath [OPTION]... [MODE-ARG]...' # Short help message in response to '-h'. usage_message="Options: --config show all configuration variables --debug enable verbose shell tracing -n, --dry-run display commands without modifying any files --features display basic configuration information and exit --mode=MODE use operation mode MODE --no-warnings equivalent to '-Wnone' --preserve-dup-deps don't remove duplicate dependency libraries --quiet, --silent don't print informational messages --tag=TAG use configuration variables from tag TAG -v, --verbose print more informational messages than default --version print version information -W, --warnings=CATEGORY report the warnings falling in CATEGORY [all] -h, --help, --help-all print short, long, or detailed help message " # Additional text appended to 'usage_message' in response to '--help'. func_help () { $debug_cmd func_usage_message $ECHO "$long_help_message MODE must be one of the following: clean remove files from the build directory compile compile a source file into a libtool object execute automatically set library path, then run a program finish complete the installation of libtool libraries install install libraries or executables link create a library or an executable uninstall remove libraries from an installed directory MODE-ARGS vary depending on the MODE. When passed as first option, '--mode=MODE' may be abbreviated as 'MODE' or a unique abbreviation of that. Try '$progname --help --mode=MODE' for a more detailed description of MODE. When reporting a bug, please describe a test case to reproduce it and include the following information: host-triplet: $host shell: $SHELL compiler: $LTCC compiler flags: $LTCFLAGS linker: $LD (gnu? $with_gnu_ld) version: $progname (GNU libtool) 2.4.6 automake: `($AUTOMAKE --version) 2>/dev/null |$SED 1q` autoconf: `($AUTOCONF --version) 2>/dev/null |$SED 1q` Report bugs to <bug-libtool@gnu.org>. GNU libtool home page: <http://www.gnu.org/software/libtool/>. General help using GNU software: <http://www.gnu.org/gethelp/>." exit 0 } # func_lo2o OBJECT-NAME # --------------------- # Transform OBJECT-NAME from a '.lo' suffix to the platform specific # object suffix. lo2o=s/\\.lo\$/.$objext/ o2lo=s/\\.$objext\$/.lo/ if test yes = "$_G_HAVE_XSI_OPS"; then eval 'func_lo2o () { case $1 in *.lo) func_lo2o_result=${1%.lo}.$objext ;; * ) func_lo2o_result=$1 ;; esac }' # func_xform LIBOBJ-OR-SOURCE # --------------------------- # Transform LIBOBJ-OR-SOURCE from a '.o' or '.c' (or otherwise) # suffix to a '.lo' libtool-object suffix. eval 'func_xform () { func_xform_result=${1%.*}.lo }' else # ...otherwise fall back to using sed. func_lo2o () { func_lo2o_result=`$ECHO "$1" | $SED "$lo2o"` } func_xform () { func_xform_result=`$ECHO "$1" | $SED 's|\.[^.]*$|.lo|'` } fi # func_fatal_configuration ARG... # ------------------------------- # Echo program name prefixed message to standard error, followed by # a configuration failure hint, and exit. func_fatal_configuration () { func__fatal_error ${1+"$@"} \ "See the $PACKAGE documentation for more information." \ "Fatal configuration error." } # func_config # ----------- # Display the configuration for all the tags in this script. func_config () { re_begincf='^# ### BEGIN LIBTOOL' re_endcf='^# ### END LIBTOOL' # Default configuration. $SED "1,/$re_begincf CONFIG/d;/$re_endcf CONFIG/,\$d" < "$progpath" # Now print the configurations for the tags. for tagname in $taglist; do $SED -n "/$re_begincf TAG CONFIG: $tagname\$/,/$re_endcf TAG CONFIG: $tagname\$/p" < "$progpath" done exit $? } # func_features # ------------- # Display the features supported by this script. func_features () { echo "host: $host" if test yes = "$build_libtool_libs"; then echo "enable shared libraries" else echo "disable shared libraries" fi if test yes = "$build_old_libs"; then echo "enable static libraries" else echo "disable static libraries" fi exit $? } # func_enable_tag TAGNAME # ----------------------- # Verify that TAGNAME is valid, and either flag an error and exit, or # enable the TAGNAME tag. We also add TAGNAME to the global $taglist # variable here. func_enable_tag () { # Global variable: tagname=$1 re_begincf="^# ### BEGIN LIBTOOL TAG CONFIG: $tagname\$" re_endcf="^# ### END LIBTOOL TAG CONFIG: $tagname\$" sed_extractcf=/$re_begincf/,/$re_endcf/p # Validate tagname. case $tagname in *[!-_A-Za-z0-9,/]*) func_fatal_error "invalid tag name: $tagname" ;; esac # Don't test for the "default" C tag, as we know it's # there but not specially marked. case $tagname in CC) ;; *) if $GREP "$re_begincf" "$progpath" >/dev/null 2>&1; then taglist="$taglist $tagname" # Evaluate the configuration. Be careful to quote the path # and the sed script, to avoid splitting on whitespace, but # also don't use non-portable quotes within backquotes within # quotes we have to do it in 2 steps: extractedcf=`$SED -n -e "$sed_extractcf" < "$progpath"` eval "$extractedcf" else func_error "ignoring unknown tag $tagname" fi ;; esac } # func_check_version_match # ------------------------ # Ensure that we are using m4 macros, and libtool script from the same # release of libtool. func_check_version_match () { if test "$package_revision" != "$macro_revision"; then if test "$VERSION" != "$macro_version"; then if test -z "$macro_version"; then cat >&2 <<_LT_EOF $progname: Version mismatch error. This is $PACKAGE $VERSION, but the $progname: definition of this LT_INIT comes from an older release. $progname: You should recreate aclocal.m4 with macros from $PACKAGE $VERSION $progname: and run autoconf again. _LT_EOF else cat >&2 <<_LT_EOF $progname: Version mismatch error. This is $PACKAGE $VERSION, but the $progname: definition of this LT_INIT comes from $PACKAGE $macro_version. $progname: You should recreate aclocal.m4 with macros from $PACKAGE $VERSION $progname: and run autoconf again. _LT_EOF fi else cat >&2 <<_LT_EOF $progname: Version mismatch error. This is $PACKAGE $VERSION, revision $package_revision, $progname: but the definition of this LT_INIT comes from revision $macro_revision. $progname: You should recreate aclocal.m4 with macros from revision $package_revision $progname: of $PACKAGE $VERSION and run autoconf again. _LT_EOF fi exit $EXIT_MISMATCH fi } # libtool_options_prep [ARG]... # ----------------------------- # Preparation for options parsed by libtool. libtool_options_prep () { $debug_mode # Option defaults: opt_config=false opt_dlopen= opt_dry_run=false opt_help=false opt_mode= opt_preserve_dup_deps=false opt_quiet=false nonopt= preserve_args= # Shorthand for --mode=foo, only valid as the first argument case $1 in clean|clea|cle|cl) shift; set dummy --mode clean ${1+"$@"}; shift ;; compile|compil|compi|comp|com|co|c) shift; set dummy --mode compile ${1+"$@"}; shift ;; execute|execut|execu|exec|exe|ex|e) shift; set dummy --mode execute ${1+"$@"}; shift ;; finish|finis|fini|fin|fi|f) shift; set dummy --mode finish ${1+"$@"}; shift ;; install|instal|insta|inst|ins|in|i) shift; set dummy --mode install ${1+"$@"}; shift ;; link|lin|li|l) shift; set dummy --mode link ${1+"$@"}; shift ;; uninstall|uninstal|uninsta|uninst|unins|unin|uni|un|u) shift; set dummy --mode uninstall ${1+"$@"}; shift ;; esac # Pass back the list of options. func_quote_for_eval ${1+"$@"} libtool_options_prep_result=$func_quote_for_eval_result } func_add_hook func_options_prep libtool_options_prep # libtool_parse_options [ARG]... # --------------------------------- # Provide handling for libtool specific options. libtool_parse_options () { $debug_cmd # Perform our own loop to consume as many options as possible in # each iteration. while test $# -gt 0; do _G_opt=$1 shift case $_G_opt in --dry-run|--dryrun|-n) opt_dry_run=: ;; --config) func_config ;; --dlopen|-dlopen) opt_dlopen="${opt_dlopen+$opt_dlopen }$1" shift ;; --preserve-dup-deps) opt_preserve_dup_deps=: ;; --features) func_features ;; --finish) set dummy --mode finish ${1+"$@"}; shift ;; --help) opt_help=: ;; --help-all) opt_help=': help-all' ;; --mode) test $# = 0 && func_missing_arg $_G_opt && break opt_mode=$1 case $1 in # Valid mode arguments: clean|compile|execute|finish|install|link|relink|uninstall) ;; # Catch anything else as an error *) func_error "invalid argument for $_G_opt" exit_cmd=exit break ;; esac shift ;; --no-silent|--no-quiet) opt_quiet=false func_append preserve_args " $_G_opt" ;; --no-warnings|--no-warning|--no-warn) opt_warning=false func_append preserve_args " $_G_opt" ;; --no-verbose) opt_verbose=false func_append preserve_args " $_G_opt" ;; --silent|--quiet) opt_quiet=: opt_verbose=false func_append preserve_args " $_G_opt" ;; --tag) test $# = 0 && func_missing_arg $_G_opt && break opt_tag=$1 func_append preserve_args " $_G_opt $1" func_enable_tag "$1" shift ;; --verbose|-v) opt_quiet=false opt_verbose=: func_append preserve_args " $_G_opt" ;; # An option not handled by this hook function: *) set dummy "$_G_opt" ${1+"$@"}; shift; break ;; esac done # save modified positional parameters for caller func_quote_for_eval ${1+"$@"} libtool_parse_options_result=$func_quote_for_eval_result } func_add_hook func_parse_options libtool_parse_options # libtool_validate_options [ARG]... # --------------------------------- # Perform any sanity checks on option settings and/or unconsumed # arguments. libtool_validate_options () { # save first non-option argument if test 0 -lt $#; then nonopt=$1 shift fi # preserve --debug test : = "$debug_cmd" || func_append preserve_args " --debug" case $host in # Solaris2 added to fix http://debbugs.gnu.org/cgi/bugreport.cgi?bug=16452 # see also: http://gcc.gnu.org/bugzilla/show_bug.cgi?id=59788 *cygwin* | *mingw* | *pw32* | *cegcc* | *solaris2* | *os2*) # don't eliminate duplications in $postdeps and $predeps opt_duplicate_compiler_generated_deps=: ;; *) opt_duplicate_compiler_generated_deps=$opt_preserve_dup_deps ;; esac $opt_help || { # Sanity checks first: func_check_version_match test yes != "$build_libtool_libs" \ && test yes != "$build_old_libs" \ && func_fatal_configuration "not configured to build any kind of library" # Darwin sucks eval std_shrext=\"$shrext_cmds\" # Only execute mode is allowed to have -dlopen flags. if test -n "$opt_dlopen" && test execute != "$opt_mode"; then func_error "unrecognized option '-dlopen'" $ECHO "$help" 1>&2 exit $EXIT_FAILURE fi # Change the help message to a mode-specific one. generic_help=$help help="Try '$progname --help --mode=$opt_mode' for more information." } # Pass back the unparsed argument list func_quote_for_eval ${1+"$@"} libtool_validate_options_result=$func_quote_for_eval_result } func_add_hook func_validate_options libtool_validate_options # Process options as early as possible so that --help and --version # can return quickly. func_options ${1+"$@"} eval set dummy "$func_options_result"; shift ## ----------- ## ## Main. ## ## ----------- ## magic='%%%MAGIC variable%%%' magic_exe='%%%MAGIC EXE variable%%%' # Global variables. extracted_archives= extracted_serial=0 # If this variable is set in any of the actions, the command in it # will be execed at the end. This prevents here-documents from being # left over by shells. exec_cmd= # A function that is used when there is no print builtin or printf. func_fallback_echo () { eval 'cat <<_LTECHO_EOF $1 _LTECHO_EOF' } # func_generated_by_libtool # True iff stdin has been generated by Libtool. This function is only # a basic sanity check; it will hardly flush out determined imposters. func_generated_by_libtool_p () { $GREP "^# Generated by .*$PACKAGE" > /dev/null 2>&1 } # func_lalib_p file # True iff FILE is a libtool '.la' library or '.lo' object file. # This function is only a basic sanity check; it will hardly flush out # determined imposters. func_lalib_p () { test -f "$1" && $SED -e 4q "$1" 2>/dev/null | func_generated_by_libtool_p } # func_lalib_unsafe_p file # True iff FILE is a libtool '.la' library or '.lo' object file. # This function implements the same check as func_lalib_p without # resorting to external programs. To this end, it redirects stdin and # closes it afterwards, without saving the original file descriptor. # As a safety measure, use it only where a negative result would be # fatal anyway. Works if 'file' does not exist. func_lalib_unsafe_p () { lalib_p=no if test -f "$1" && test -r "$1" && exec 5<&0 <"$1"; then for lalib_p_l in 1 2 3 4 do read lalib_p_line case $lalib_p_line in \#\ Generated\ by\ *$PACKAGE* ) lalib_p=yes; break;; esac done exec 0<&5 5<&- fi test yes = "$lalib_p" } # func_ltwrapper_script_p file # True iff FILE is a libtool wrapper script # This function is only a basic sanity check; it will hardly flush out # determined imposters. func_ltwrapper_script_p () { test -f "$1" && $lt_truncate_bin < "$1" 2>/dev/null | func_generated_by_libtool_p } # func_ltwrapper_executable_p file # True iff FILE is a libtool wrapper executable # This function is only a basic sanity check; it will hardly flush out # determined imposters. func_ltwrapper_executable_p () { func_ltwrapper_exec_suffix= case $1 in *.exe) ;; *) func_ltwrapper_exec_suffix=.exe ;; esac $GREP "$magic_exe" "$1$func_ltwrapper_exec_suffix" >/dev/null 2>&1 } # func_ltwrapper_scriptname file # Assumes file is an ltwrapper_executable # uses $file to determine the appropriate filename for a # temporary ltwrapper_script. func_ltwrapper_scriptname () { func_dirname_and_basename "$1" "" "." func_stripname '' '.exe' "$func_basename_result" func_ltwrapper_scriptname_result=$func_dirname_result/$objdir/${func_stripname_result}_ltshwrapper } # func_ltwrapper_p file # True iff FILE is a libtool wrapper script or wrapper executable # This function is only a basic sanity check; it will hardly flush out # determined imposters. func_ltwrapper_p () { func_ltwrapper_script_p "$1" || func_ltwrapper_executable_p "$1" } # func_execute_cmds commands fail_cmd # Execute tilde-delimited COMMANDS. # If FAIL_CMD is given, eval that upon failure. # FAIL_CMD may read-access the current command in variable CMD! func_execute_cmds () { $debug_cmd save_ifs=$IFS; IFS='~' for cmd in $1; do IFS=$sp$nl eval cmd=\"$cmd\" IFS=$save_ifs func_show_eval "$cmd" "${2-:}" done IFS=$save_ifs } # func_source file # Source FILE, adding directory component if necessary. # Note that it is not necessary on cygwin/mingw to append a dot to # FILE even if both FILE and FILE.exe exist: automatic-append-.exe # behavior happens only for exec(3), not for open(2)! Also, sourcing # 'FILE.' does not work on cygwin managed mounts. func_source () { $debug_cmd case $1 in */* | *\\*) . "$1" ;; *) . "./$1" ;; esac } # func_resolve_sysroot PATH # Replace a leading = in PATH with a sysroot. Store the result into # func_resolve_sysroot_result func_resolve_sysroot () { func_resolve_sysroot_result=$1 case $func_resolve_sysroot_result in =*) func_stripname '=' '' "$func_resolve_sysroot_result" func_resolve_sysroot_result=$lt_sysroot$func_stripname_result ;; esac } # func_replace_sysroot PATH # If PATH begins with the sysroot, replace it with = and # store the result into func_replace_sysroot_result. func_replace_sysroot () { case $lt_sysroot:$1 in ?*:"$lt_sysroot"*) func_stripname "$lt_sysroot" '' "$1" func_replace_sysroot_result='='$func_stripname_result ;; *) # Including no sysroot. func_replace_sysroot_result=$1 ;; esac } # func_infer_tag arg # Infer tagged configuration to use if any are available and # if one wasn't chosen via the "--tag" command line option. # Only attempt this if the compiler in the base compile # command doesn't match the default compiler. # arg is usually of the form 'gcc ...' func_infer_tag () { $debug_cmd if test -n "$available_tags" && test -z "$tagname"; then CC_quoted= for arg in $CC; do func_append_quoted CC_quoted "$arg" done CC_expanded=`func_echo_all $CC` CC_quoted_expanded=`func_echo_all $CC_quoted` case $@ in # Blanks in the command may have been stripped by the calling shell, # but not from the CC environment variable when configure was run. " $CC "* | "$CC "* | " $CC_expanded "* | "$CC_expanded "* | \ " $CC_quoted"* | "$CC_quoted "* | " $CC_quoted_expanded "* | "$CC_quoted_expanded "*) ;; # Blanks at the start of $base_compile will cause this to fail # if we don't check for them as well. *) for z in $available_tags; do if $GREP "^# ### BEGIN LIBTOOL TAG CONFIG: $z$" < "$progpath" > /dev/null; then # Evaluate the configuration. eval "`$SED -n -e '/^# ### BEGIN LIBTOOL TAG CONFIG: '$z'$/,/^# ### END LIBTOOL TAG CONFIG: '$z'$/p' < $progpath`" CC_quoted= for arg in $CC; do # Double-quote args containing other shell metacharacters. func_append_quoted CC_quoted "$arg" done CC_expanded=`func_echo_all $CC` CC_quoted_expanded=`func_echo_all $CC_quoted` case "$@ " in " $CC "* | "$CC "* | " $CC_expanded "* | "$CC_expanded "* | \ " $CC_quoted"* | "$CC_quoted "* | " $CC_quoted_expanded "* | "$CC_quoted_expanded "*) # The compiler in the base compile command matches # the one in the tagged configuration. # Assume this is the tagged configuration we want. tagname=$z break ;; esac fi done # If $tagname still isn't set, then no tagged configuration # was found and let the user know that the "--tag" command # line option must be used. if test -z "$tagname"; then func_echo "unable to infer tagged configuration" func_fatal_error "specify a tag with '--tag'" # else # func_verbose "using $tagname tagged configuration" fi ;; esac fi } # func_write_libtool_object output_name pic_name nonpic_name # Create a libtool object file (analogous to a ".la" file), # but don't create it if we're doing a dry run. func_write_libtool_object () { write_libobj=$1 if test yes = "$build_libtool_libs"; then write_lobj=\'$2\' else write_lobj=none fi if test yes = "$build_old_libs"; then write_oldobj=\'$3\' else write_oldobj=none fi $opt_dry_run || { cat >${write_libobj}T <<EOF # $write_libobj - a libtool object file # Generated by $PROGRAM (GNU $PACKAGE) $VERSION # # Please DO NOT delete this file! # It is necessary for linking the library. # Name of the PIC object. pic_object=$write_lobj # Name of the non-PIC object non_pic_object=$write_oldobj EOF $MV "${write_libobj}T" "$write_libobj" } } ################################################## # FILE NAME AND PATH CONVERSION HELPER FUNCTIONS # ################################################## # func_convert_core_file_wine_to_w32 ARG # Helper function used by file name conversion functions when $build is *nix, # and $host is mingw, cygwin, or some other w32 environment. Relies on a # correctly configured wine environment available, with the winepath program # in $build's $PATH. # # ARG is the $build file name to be converted to w32 format. # Result is available in $func_convert_core_file_wine_to_w32_result, and will # be empty on error (or when ARG is empty) func_convert_core_file_wine_to_w32 () { $debug_cmd func_convert_core_file_wine_to_w32_result=$1 if test -n "$1"; then # Unfortunately, winepath does not exit with a non-zero error code, so we # are forced to check the contents of stdout. On the other hand, if the # command is not found, the shell will set an exit code of 127 and print # *an error message* to stdout. So we must check for both error code of # zero AND non-empty stdout, which explains the odd construction: func_convert_core_file_wine_to_w32_tmp=`winepath -w "$1" 2>/dev/null` if test "$?" -eq 0 && test -n "$func_convert_core_file_wine_to_w32_tmp"; then func_convert_core_file_wine_to_w32_result=`$ECHO "$func_convert_core_file_wine_to_w32_tmp" | $SED -e "$sed_naive_backslashify"` else func_convert_core_file_wine_to_w32_result= fi fi } # end: func_convert_core_file_wine_to_w32 # func_convert_core_path_wine_to_w32 ARG # Helper function used by path conversion functions when $build is *nix, and # $host is mingw, cygwin, or some other w32 environment. Relies on a correctly # configured wine environment available, with the winepath program in $build's # $PATH. Assumes ARG has no leading or trailing path separator characters. # # ARG is path to be converted from $build format to win32. # Result is available in $func_convert_core_path_wine_to_w32_result. # Unconvertible file (directory) names in ARG are skipped; if no directory names # are convertible, then the result may be empty. func_convert_core_path_wine_to_w32 () { $debug_cmd # unfortunately, winepath doesn't convert paths, only file names func_convert_core_path_wine_to_w32_result= if test -n "$1"; then oldIFS=$IFS IFS=: for func_convert_core_path_wine_to_w32_f in $1; do IFS=$oldIFS func_convert_core_file_wine_to_w32 "$func_convert_core_path_wine_to_w32_f" if test -n "$func_convert_core_file_wine_to_w32_result"; then if test -z "$func_convert_core_path_wine_to_w32_result"; then func_convert_core_path_wine_to_w32_result=$func_convert_core_file_wine_to_w32_result else func_append func_convert_core_path_wine_to_w32_result ";$func_convert_core_file_wine_to_w32_result" fi fi done IFS=$oldIFS fi } # end: func_convert_core_path_wine_to_w32 # func_cygpath ARGS... # Wrapper around calling the cygpath program via LT_CYGPATH. This is used when # when (1) $build is *nix and Cygwin is hosted via a wine environment; or (2) # $build is MSYS and $host is Cygwin, or (3) $build is Cygwin. In case (1) or # (2), returns the Cygwin file name or path in func_cygpath_result (input # file name or path is assumed to be in w32 format, as previously converted # from $build's *nix or MSYS format). In case (3), returns the w32 file name # or path in func_cygpath_result (input file name or path is assumed to be in # Cygwin format). Returns an empty string on error. # # ARGS are passed to cygpath, with the last one being the file name or path to # be converted. # # Specify the absolute *nix (or w32) name to cygpath in the LT_CYGPATH # environment variable; do not put it in $PATH. func_cygpath () { $debug_cmd if test -n "$LT_CYGPATH" && test -f "$LT_CYGPATH"; then func_cygpath_result=`$LT_CYGPATH "$@" 2>/dev/null` if test "$?" -ne 0; then # on failure, ensure result is empty func_cygpath_result= fi else func_cygpath_result= func_error "LT_CYGPATH is empty or specifies non-existent file: '$LT_CYGPATH'" fi } #end: func_cygpath # func_convert_core_msys_to_w32 ARG # Convert file name or path ARG from MSYS format to w32 format. Return # result in func_convert_core_msys_to_w32_result. func_convert_core_msys_to_w32 () { $debug_cmd # awkward: cmd appends spaces to result func_convert_core_msys_to_w32_result=`( cmd //c echo "$1" ) 2>/dev/null | $SED -e 's/[ ]*$//' -e "$sed_naive_backslashify"` } #end: func_convert_core_msys_to_w32 # func_convert_file_check ARG1 ARG2 # Verify that ARG1 (a file name in $build format) was converted to $host # format in ARG2. Otherwise, emit an error message, but continue (resetting # func_to_host_file_result to ARG1). func_convert_file_check () { $debug_cmd if test -z "$2" && test -n "$1"; then func_error "Could not determine host file name corresponding to" func_error " '$1'" func_error "Continuing, but uninstalled executables may not work." # Fallback: func_to_host_file_result=$1 fi } # end func_convert_file_check # func_convert_path_check FROM_PATHSEP TO_PATHSEP FROM_PATH TO_PATH # Verify that FROM_PATH (a path in $build format) was converted to $host # format in TO_PATH. Otherwise, emit an error message, but continue, resetting # func_to_host_file_result to a simplistic fallback value (see below). func_convert_path_check () { $debug_cmd if test -z "$4" && test -n "$3"; then func_error "Could not determine the host path corresponding to" func_error " '$3'" func_error "Continuing, but uninstalled executables may not work." # Fallback. This is a deliberately simplistic "conversion" and # should not be "improved". See libtool.info. if test "x$1" != "x$2"; then lt_replace_pathsep_chars="s|$1|$2|g" func_to_host_path_result=`echo "$3" | $SED -e "$lt_replace_pathsep_chars"` else func_to_host_path_result=$3 fi fi } # end func_convert_path_check # func_convert_path_front_back_pathsep FRONTPAT BACKPAT REPL ORIG # Modifies func_to_host_path_result by prepending REPL if ORIG matches FRONTPAT # and appending REPL if ORIG matches BACKPAT. func_convert_path_front_back_pathsep () { $debug_cmd case $4 in $1 ) func_to_host_path_result=$3$func_to_host_path_result ;; esac case $4 in $2 ) func_append func_to_host_path_result "$3" ;; esac } # end func_convert_path_front_back_pathsep ################################################## # $build to $host FILE NAME CONVERSION FUNCTIONS # ################################################## # invoked via '$to_host_file_cmd ARG' # # In each case, ARG is the path to be converted from $build to $host format. # Result will be available in $func_to_host_file_result. # func_to_host_file ARG # Converts the file name ARG from $build format to $host format. Return result # in func_to_host_file_result. func_to_host_file () { $debug_cmd $to_host_file_cmd "$1" } # end func_to_host_file # func_to_tool_file ARG LAZY # converts the file name ARG from $build format to toolchain format. Return # result in func_to_tool_file_result. If the conversion in use is listed # in (the comma separated) LAZY, no conversion takes place. func_to_tool_file () { $debug_cmd case ,$2, in *,"$to_tool_file_cmd",*) func_to_tool_file_result=$1 ;; *) $to_tool_file_cmd "$1" func_to_tool_file_result=$func_to_host_file_result ;; esac } # end func_to_tool_file # func_convert_file_noop ARG # Copy ARG to func_to_host_file_result. func_convert_file_noop () { func_to_host_file_result=$1 } # end func_convert_file_noop # func_convert_file_msys_to_w32 ARG # Convert file name ARG from (mingw) MSYS to (mingw) w32 format; automatic # conversion to w32 is not available inside the cwrapper. Returns result in # func_to_host_file_result. func_convert_file_msys_to_w32 () { $debug_cmd func_to_host_file_result=$1 if test -n "$1"; then func_convert_core_msys_to_w32 "$1" func_to_host_file_result=$func_convert_core_msys_to_w32_result fi func_convert_file_check "$1" "$func_to_host_file_result" } # end func_convert_file_msys_to_w32 # func_convert_file_cygwin_to_w32 ARG # Convert file name ARG from Cygwin to w32 format. Returns result in # func_to_host_file_result. func_convert_file_cygwin_to_w32 () { $debug_cmd func_to_host_file_result=$1 if test -n "$1"; then # because $build is cygwin, we call "the" cygpath in $PATH; no need to use # LT_CYGPATH in this case. func_to_host_file_result=`cygpath -m "$1"` fi func_convert_file_check "$1" "$func_to_host_file_result" } # end func_convert_file_cygwin_to_w32 # func_convert_file_nix_to_w32 ARG # Convert file name ARG from *nix to w32 format. Requires a wine environment # and a working winepath. Returns result in func_to_host_file_result. func_convert_file_nix_to_w32 () { $debug_cmd func_to_host_file_result=$1 if test -n "$1"; then func_convert_core_file_wine_to_w32 "$1" func_to_host_file_result=$func_convert_core_file_wine_to_w32_result fi func_convert_file_check "$1" "$func_to_host_file_result" } # end func_convert_file_nix_to_w32 # func_convert_file_msys_to_cygwin ARG # Convert file name ARG from MSYS to Cygwin format. Requires LT_CYGPATH set. # Returns result in func_to_host_file_result. func_convert_file_msys_to_cygwin () { $debug_cmd func_to_host_file_result=$1 if test -n "$1"; then func_convert_core_msys_to_w32 "$1" func_cygpath -u "$func_convert_core_msys_to_w32_result" func_to_host_file_result=$func_cygpath_result fi func_convert_file_check "$1" "$func_to_host_file_result" } # end func_convert_file_msys_to_cygwin # func_convert_file_nix_to_cygwin ARG # Convert file name ARG from *nix to Cygwin format. Requires Cygwin installed # in a wine environment, working winepath, and LT_CYGPATH set. Returns result # in func_to_host_file_result. func_convert_file_nix_to_cygwin () { $debug_cmd func_to_host_file_result=$1 if test -n "$1"; then # convert from *nix to w32, then use cygpath to convert from w32 to cygwin. func_convert_core_file_wine_to_w32 "$1" func_cygpath -u "$func_convert_core_file_wine_to_w32_result" func_to_host_file_result=$func_cygpath_result fi func_convert_file_check "$1" "$func_to_host_file_result" } # end func_convert_file_nix_to_cygwin ############################################# # $build to $host PATH CONVERSION FUNCTIONS # ############################################# # invoked via '$to_host_path_cmd ARG' # # In each case, ARG is the path to be converted from $build to $host format. # The result will be available in $func_to_host_path_result. # # Path separators are also converted from $build format to $host format. If # ARG begins or ends with a path separator character, it is preserved (but # converted to $host format) on output. # # All path conversion functions are named using the following convention: # file name conversion function : func_convert_file_X_to_Y () # path conversion function : func_convert_path_X_to_Y () # where, for any given $build/$host combination the 'X_to_Y' value is the # same. If conversion functions are added for new $build/$host combinations, # the two new functions must follow this pattern, or func_init_to_host_path_cmd # will break. # func_init_to_host_path_cmd # Ensures that function "pointer" variable $to_host_path_cmd is set to the # appropriate value, based on the value of $to_host_file_cmd. to_host_path_cmd= func_init_to_host_path_cmd () { $debug_cmd if test -z "$to_host_path_cmd"; then func_stripname 'func_convert_file_' '' "$to_host_file_cmd" to_host_path_cmd=func_convert_path_$func_stripname_result fi } # func_to_host_path ARG # Converts the path ARG from $build format to $host format. Return result # in func_to_host_path_result. func_to_host_path () { $debug_cmd func_init_to_host_path_cmd $to_host_path_cmd "$1" } # end func_to_host_path # func_convert_path_noop ARG # Copy ARG to func_to_host_path_result. func_convert_path_noop () { func_to_host_path_result=$1 } # end func_convert_path_noop # func_convert_path_msys_to_w32 ARG # Convert path ARG from (mingw) MSYS to (mingw) w32 format; automatic # conversion to w32 is not available inside the cwrapper. Returns result in # func_to_host_path_result. func_convert_path_msys_to_w32 () { $debug_cmd func_to_host_path_result=$1 if test -n "$1"; then # Remove leading and trailing path separator characters from ARG. MSYS # behavior is inconsistent here; cygpath turns them into '.;' and ';.'; # and winepath ignores them completely. func_stripname : : "$1" func_to_host_path_tmp1=$func_stripname_result func_convert_core_msys_to_w32 "$func_to_host_path_tmp1" func_to_host_path_result=$func_convert_core_msys_to_w32_result func_convert_path_check : ";" \ "$func_to_host_path_tmp1" "$func_to_host_path_result" func_convert_path_front_back_pathsep ":*" "*:" ";" "$1" fi } # end func_convert_path_msys_to_w32 # func_convert_path_cygwin_to_w32 ARG # Convert path ARG from Cygwin to w32 format. Returns result in # func_to_host_file_result. func_convert_path_cygwin_to_w32 () { $debug_cmd func_to_host_path_result=$1 if test -n "$1"; then # See func_convert_path_msys_to_w32: func_stripname : : "$1" func_to_host_path_tmp1=$func_stripname_result func_to_host_path_result=`cygpath -m -p "$func_to_host_path_tmp1"` func_convert_path_check : ";" \ "$func_to_host_path_tmp1" "$func_to_host_path_result" func_convert_path_front_back_pathsep ":*" "*:" ";" "$1" fi } # end func_convert_path_cygwin_to_w32 # func_convert_path_nix_to_w32 ARG # Convert path ARG from *nix to w32 format. Requires a wine environment and # a working winepath. Returns result in func_to_host_file_result. func_convert_path_nix_to_w32 () { $debug_cmd func_to_host_path_result=$1 if test -n "$1"; then # See func_convert_path_msys_to_w32: func_stripname : : "$1" func_to_host_path_tmp1=$func_stripname_result func_convert_core_path_wine_to_w32 "$func_to_host_path_tmp1" func_to_host_path_result=$func_convert_core_path_wine_to_w32_result func_convert_path_check : ";" \ "$func_to_host_path_tmp1" "$func_to_host_path_result" func_convert_path_front_back_pathsep ":*" "*:" ";" "$1" fi } # end func_convert_path_nix_to_w32 # func_convert_path_msys_to_cygwin ARG # Convert path ARG from MSYS to Cygwin format. Requires LT_CYGPATH set. # Returns result in func_to_host_file_result. func_convert_path_msys_to_cygwin () { $debug_cmd func_to_host_path_result=$1 if test -n "$1"; then # See func_convert_path_msys_to_w32: func_stripname : : "$1" func_to_host_path_tmp1=$func_stripname_result func_convert_core_msys_to_w32 "$func_to_host_path_tmp1" func_cygpath -u -p "$func_convert_core_msys_to_w32_result" func_to_host_path_result=$func_cygpath_result func_convert_path_check : : \ "$func_to_host_path_tmp1" "$func_to_host_path_result" func_convert_path_front_back_pathsep ":*" "*:" : "$1" fi } # end func_convert_path_msys_to_cygwin # func_convert_path_nix_to_cygwin ARG # Convert path ARG from *nix to Cygwin format. Requires Cygwin installed in a # a wine environment, working winepath, and LT_CYGPATH set. Returns result in # func_to_host_file_result. func_convert_path_nix_to_cygwin () { $debug_cmd func_to_host_path_result=$1 if test -n "$1"; then # Remove leading and trailing path separator characters from # ARG. msys behavior is inconsistent here, cygpath turns them # into '.;' and ';.', and winepath ignores them completely. func_stripname : : "$1" func_to_host_path_tmp1=$func_stripname_result func_convert_core_path_wine_to_w32 "$func_to_host_path_tmp1" func_cygpath -u -p "$func_convert_core_path_wine_to_w32_result" func_to_host_path_result=$func_cygpath_result func_convert_path_check : : \ "$func_to_host_path_tmp1" "$func_to_host_path_result" func_convert_path_front_back_pathsep ":*" "*:" : "$1" fi } # end func_convert_path_nix_to_cygwin # func_dll_def_p FILE # True iff FILE is a Windows DLL '.def' file. # Keep in sync with _LT_DLL_DEF_P in libtool.m4 func_dll_def_p () { $debug_cmd func_dll_def_p_tmp=`$SED -n \ -e 's/^[ ]*//' \ -e '/^\(;.*\)*$/d' \ -e 's/^\(EXPORTS\|LIBRARY\)\([ ].*\)*$/DEF/p' \ -e q \ "$1"` test DEF = "$func_dll_def_p_tmp" } # func_mode_compile arg... func_mode_compile () { $debug_cmd # Get the compilation command and the source file. base_compile= srcfile=$nonopt # always keep a non-empty value in "srcfile" suppress_opt=yes suppress_output= arg_mode=normal libobj= later= pie_flag= for arg do case $arg_mode in arg ) # do not "continue". Instead, add this to base_compile lastarg=$arg arg_mode=normal ;; target ) libobj=$arg arg_mode=normal continue ;; normal ) # Accept any command-line options. case $arg in -o) test -n "$libobj" && \ func_fatal_error "you cannot specify '-o' more than once" arg_mode=target continue ;; -pie | -fpie | -fPIE) func_append pie_flag " $arg" continue ;; -shared | -static | -prefer-pic | -prefer-non-pic) func_append later " $arg" continue ;; -no-suppress) suppress_opt=no continue ;; -Xcompiler) arg_mode=arg # the next one goes into the "base_compile" arg list continue # The current "srcfile" will either be retained or ;; # replaced later. I would guess that would be a bug. -Wc,*) func_stripname '-Wc,' '' "$arg" args=$func_stripname_result lastarg= save_ifs=$IFS; IFS=, for arg in $args; do IFS=$save_ifs func_append_quoted lastarg "$arg" done IFS=$save_ifs func_stripname ' ' '' "$lastarg" lastarg=$func_stripname_result # Add the arguments to base_compile. func_append base_compile " $lastarg" continue ;; *) # Accept the current argument as the source file. # The previous "srcfile" becomes the current argument. # lastarg=$srcfile srcfile=$arg ;; esac # case $arg ;; esac # case $arg_mode # Aesthetically quote the previous argument. func_append_quoted base_compile "$lastarg" done # for arg case $arg_mode in arg) func_fatal_error "you must specify an argument for -Xcompile" ;; target) func_fatal_error "you must specify a target with '-o'" ;; *) # Get the name of the library object. test -z "$libobj" && { func_basename "$srcfile" libobj=$func_basename_result } ;; esac # Recognize several different file suffixes. # If the user specifies -o file.o, it is replaced with file.lo case $libobj in *.[cCFSifmso] | \ *.ada | *.adb | *.ads | *.asm | \ *.c++ | *.cc | *.ii | *.class | *.cpp | *.cxx | \ *.[fF][09]? | *.for | *.java | *.go | *.obj | *.sx | *.cu | *.cup) func_xform "$libobj" libobj=$func_xform_result ;; esac case $libobj in *.lo) func_lo2o "$libobj"; obj=$func_lo2o_result ;; *) func_fatal_error "cannot determine name of library object from '$libobj'" ;; esac func_infer_tag $base_compile for arg in $later; do case $arg in -shared) test yes = "$build_libtool_libs" \ || func_fatal_configuration "cannot build a shared library" build_old_libs=no continue ;; -static) build_libtool_libs=no build_old_libs=yes continue ;; -prefer-pic) pic_mode=yes continue ;; -prefer-non-pic) pic_mode=no continue ;; esac done func_quote_for_eval "$libobj" test "X$libobj" != "X$func_quote_for_eval_result" \ && $ECHO "X$libobj" | $GREP '[]~#^*{};<>?"'"'"' &()|`$[]' \ && func_warning "libobj name '$libobj' may not contain shell special characters." func_dirname_and_basename "$obj" "/" "" objname=$func_basename_result xdir=$func_dirname_result lobj=$xdir$objdir/$objname test -z "$base_compile" && \ func_fatal_help "you must specify a compilation command" # Delete any leftover library objects. if test yes = "$build_old_libs"; then removelist="$obj $lobj $libobj ${libobj}T" else removelist="$lobj $libobj ${libobj}T" fi # On Cygwin there's no "real" PIC flag so we must build both object types case $host_os in cygwin* | mingw* | pw32* | os2* | cegcc*) pic_mode=default ;; esac if test no = "$pic_mode" && test pass_all != "$deplibs_check_method"; then # non-PIC code in shared libraries is not supported pic_mode=default fi # Calculate the filename of the output object if compiler does # not support -o with -c if test no = "$compiler_c_o"; then output_obj=`$ECHO "$srcfile" | $SED 's%^.*/%%; s%\.[^.]*$%%'`.$objext lockfile=$output_obj.lock else output_obj= need_locks=no lockfile= fi # Lock this critical section if it is needed # We use this script file to make the link, it avoids creating a new file if test yes = "$need_locks"; then until $opt_dry_run || ln "$progpath" "$lockfile" 2>/dev/null; do func_echo "Waiting for $lockfile to be removed" sleep 2 done elif test warn = "$need_locks"; then if test -f "$lockfile"; then $ECHO "\ *** ERROR, $lockfile exists and contains: `cat $lockfile 2>/dev/null` This indicates that another process is trying to use the same temporary object file, and libtool could not work around it because your compiler does not support '-c' and '-o' together. If you repeat this compilation, it may succeed, by chance, but you had better avoid parallel builds (make -j) in this platform, or get a better compiler." $opt_dry_run || $RM $removelist exit $EXIT_FAILURE fi func_append removelist " $output_obj" $ECHO "$srcfile" > "$lockfile" fi $opt_dry_run || $RM $removelist func_append removelist " $lockfile" trap '$opt_dry_run || $RM $removelist; exit $EXIT_FAILURE' 1 2 15 func_to_tool_file "$srcfile" func_convert_file_msys_to_w32 srcfile=$func_to_tool_file_result func_quote_for_eval "$srcfile" qsrcfile=$func_quote_for_eval_result # Only build a PIC object if we are building libtool libraries. if test yes = "$build_libtool_libs"; then # Without this assignment, base_compile gets emptied. fbsd_hideous_sh_bug=$base_compile if test no != "$pic_mode"; then command="$base_compile $qsrcfile $pic_flag" else # Don't build PIC code command="$base_compile $qsrcfile" fi func_mkdir_p "$xdir$objdir" if test -z "$output_obj"; then # Place PIC objects in $objdir func_append command " -o $lobj" fi func_show_eval_locale "$command" \ 'test -n "$output_obj" && $RM $removelist; exit $EXIT_FAILURE' if test warn = "$need_locks" && test "X`cat $lockfile 2>/dev/null`" != "X$srcfile"; then $ECHO "\ *** ERROR, $lockfile contains: `cat $lockfile 2>/dev/null` but it should contain: $srcfile This indicates that another process is trying to use the same temporary object file, and libtool could not work around it because your compiler does not support '-c' and '-o' together. If you repeat this compilation, it may succeed, by chance, but you had better avoid parallel builds (make -j) in this platform, or get a better compiler." $opt_dry_run || $RM $removelist exit $EXIT_FAILURE fi # Just move the object if needed, then go on to compile the next one if test -n "$output_obj" && test "X$output_obj" != "X$lobj"; then func_show_eval '$MV "$output_obj" "$lobj"' \ 'error=$?; $opt_dry_run || $RM $removelist; exit $error' fi # Allow error messages only from the first compilation. if test yes = "$suppress_opt"; then suppress_output=' >/dev/null 2>&1' fi fi # Only build a position-dependent object if we build old libraries. if test yes = "$build_old_libs"; then if test yes != "$pic_mode"; then # Don't build PIC code command="$base_compile $qsrcfile$pie_flag" else command="$base_compile $qsrcfile $pic_flag" fi if test yes = "$compiler_c_o"; then func_append command " -o $obj" fi # Suppress compiler output if we already did a PIC compilation. func_append command "$suppress_output" func_show_eval_locale "$command" \ '$opt_dry_run || $RM $removelist; exit $EXIT_FAILURE' if test warn = "$need_locks" && test "X`cat $lockfile 2>/dev/null`" != "X$srcfile"; then $ECHO "\ *** ERROR, $lockfile contains: `cat $lockfile 2>/dev/null` but it should contain: $srcfile This indicates that another process is trying to use the same temporary object file, and libtool could not work around it because your compiler does not support '-c' and '-o' together. If you repeat this compilation, it may succeed, by chance, but you had better avoid parallel builds (make -j) in this platform, or get a better compiler." $opt_dry_run || $RM $removelist exit $EXIT_FAILURE fi # Just move the object if needed if test -n "$output_obj" && test "X$output_obj" != "X$obj"; then func_show_eval '$MV "$output_obj" "$obj"' \ 'error=$?; $opt_dry_run || $RM $removelist; exit $error' fi fi $opt_dry_run || { func_write_libtool_object "$libobj" "$objdir/$objname" "$objname" # Unlock the critical section if it was locked if test no != "$need_locks"; then removelist=$lockfile $RM "$lockfile" fi } exit $EXIT_SUCCESS } $opt_help || { test compile = "$opt_mode" && func_mode_compile ${1+"$@"} } func_mode_help () { # We need to display help for each of the modes. case $opt_mode in "") # Generic help is extracted from the usage comments # at the start of this file. func_help ;; clean) $ECHO \ "Usage: $progname [OPTION]... --mode=clean RM [RM-OPTION]... FILE... Remove files from the build directory. RM is the name of the program to use to delete files associated with each FILE (typically '/bin/rm'). RM-OPTIONS are options (such as '-f') to be passed to RM. If FILE is a libtool library, object or program, all the files associated with it are deleted. Otherwise, only FILE itself is deleted using RM." ;; compile) $ECHO \ "Usage: $progname [OPTION]... --mode=compile COMPILE-COMMAND... SOURCEFILE Compile a source file into a libtool library object. This mode accepts the following additional options: -o OUTPUT-FILE set the output file name to OUTPUT-FILE -no-suppress do not suppress compiler output for multiple passes -prefer-pic try to build PIC objects only -prefer-non-pic try to build non-PIC objects only -shared do not build a '.o' file suitable for static linking -static only build a '.o' file suitable for static linking -Wc,FLAG pass FLAG directly to the compiler COMPILE-COMMAND is a command to be used in creating a 'standard' object file from the given SOURCEFILE. The output file name is determined by removing the directory component from SOURCEFILE, then substituting the C source code suffix '.c' with the library object suffix, '.lo'." ;; execute) $ECHO \ "Usage: $progname [OPTION]... --mode=execute COMMAND [ARGS]... Automatically set library path, then run a program. This mode accepts the following additional options: -dlopen FILE add the directory containing FILE to the library path This mode sets the library path environment variable according to '-dlopen' flags. If any of the ARGS are libtool executable wrappers, then they are translated into their corresponding uninstalled binary, and any of their required library directories are added to the library path. Then, COMMAND is executed, with ARGS as arguments." ;; finish) $ECHO \ "Usage: $progname [OPTION]... --mode=finish [LIBDIR]... Complete the installation of libtool libraries. Each LIBDIR is a directory that contains libtool libraries. The commands that this mode executes may require superuser privileges. Use the '--dry-run' option if you just want to see what would be executed." ;; install) $ECHO \ "Usage: $progname [OPTION]... --mode=install INSTALL-COMMAND... Install executables or libraries. INSTALL-COMMAND is the installation command. The first component should be either the 'install' or 'cp' program. The following components of INSTALL-COMMAND are treated specially: -inst-prefix-dir PREFIX-DIR Use PREFIX-DIR as a staging area for installation The rest of the components are interpreted as arguments to that command (only BSD-compatible install options are recognized)." ;; link) $ECHO \ "Usage: $progname [OPTION]... --mode=link LINK-COMMAND... Link object files or libraries together to form another library, or to create an executable program. LINK-COMMAND is a command using the C compiler that you would use to create a program from several object files. The following components of LINK-COMMAND are treated specially: -all-static do not do any dynamic linking at all -avoid-version do not add a version suffix if possible -bindir BINDIR specify path to binaries directory (for systems where libraries must be found in the PATH setting at runtime) -dlopen FILE '-dlpreopen' FILE if it cannot be dlopened at runtime -dlpreopen FILE link in FILE and add its symbols to lt_preloaded_symbols -export-dynamic allow symbols from OUTPUT-FILE to be resolved with dlsym(3) -export-symbols SYMFILE try to export only the symbols listed in SYMFILE -export-symbols-regex REGEX try to export only the symbols matching REGEX -LLIBDIR search LIBDIR for required installed libraries -lNAME OUTPUT-FILE requires the installed library libNAME -module build a library that can dlopened -no-fast-install disable the fast-install mode -no-install link a not-installable executable -no-undefined declare that a library does not refer to external symbols -o OUTPUT-FILE create OUTPUT-FILE from the specified objects -objectlist FILE use a list of object files found in FILE to specify objects -os2dllname NAME force a short DLL name on OS/2 (no effect on other OSes) -precious-files-regex REGEX don't remove output files matching REGEX -release RELEASE specify package release information -rpath LIBDIR the created library will eventually be installed in LIBDIR -R[ ]LIBDIR add LIBDIR to the runtime path of programs and libraries -shared only do dynamic linking of libtool libraries -shrext SUFFIX override the standard shared library file extension -static do not do any dynamic linking of uninstalled libtool libraries -static-libtool-libs do not do any dynamic linking of libtool libraries -version-info CURRENT[:REVISION[:AGE]] specify library version info [each variable defaults to 0] -weak LIBNAME declare that the target provides the LIBNAME interface -Wc,FLAG -Xcompiler FLAG pass linker-specific FLAG directly to the compiler -Wl,FLAG -Xlinker FLAG pass linker-specific FLAG directly to the linker -XCClinker FLAG pass link-specific FLAG to the compiler driver (CC) All other options (arguments beginning with '-') are ignored. Every other argument is treated as a filename. Files ending in '.la' are treated as uninstalled libtool libraries, other files are standard or library object files. If the OUTPUT-FILE ends in '.la', then a libtool library is created, only library objects ('.lo' files) may be specified, and '-rpath' is required, except when creating a convenience library. If OUTPUT-FILE ends in '.a' or '.lib', then a standard library is created using 'ar' and 'ranlib', or on Windows using 'lib'. If OUTPUT-FILE ends in '.lo' or '.$objext', then a reloadable object file is created, otherwise an executable program is created." ;; uninstall) $ECHO \ "Usage: $progname [OPTION]... --mode=uninstall RM [RM-OPTION]... FILE... Remove libraries from an installation directory. RM is the name of the program to use to delete files associated with each FILE (typically '/bin/rm'). RM-OPTIONS are options (such as '-f') to be passed to RM. If FILE is a libtool library, all the files associated with it are deleted. Otherwise, only FILE itself is deleted using RM." ;; *) func_fatal_help "invalid operation mode '$opt_mode'" ;; esac echo $ECHO "Try '$progname --help' for more information about other modes." } # Now that we've collected a possible --mode arg, show help if necessary if $opt_help; then if test : = "$opt_help"; then func_mode_help else { func_help noexit for opt_mode in compile link execute install finish uninstall clean; do func_mode_help done } | $SED -n '1p; 2,$s/^Usage:/ or: /p' { func_help noexit for opt_mode in compile link execute install finish uninstall clean; do echo func_mode_help done } | $SED '1d /^When reporting/,/^Report/{ H d } $x /information about other modes/d /more detailed .*MODE/d s/^Usage:.*--mode=\([^ ]*\) .*/Description of \1 mode:/' fi exit $? fi # func_mode_execute arg... func_mode_execute () { $debug_cmd # The first argument is the command name. cmd=$nonopt test -z "$cmd" && \ func_fatal_help "you must specify a COMMAND" # Handle -dlopen flags immediately. for file in $opt_dlopen; do test -f "$file" \ || func_fatal_help "'$file' is not a file" dir= case $file in *.la) func_resolve_sysroot "$file" file=$func_resolve_sysroot_result # Check to see that this really is a libtool archive. func_lalib_unsafe_p "$file" \ || func_fatal_help "'$lib' is not a valid libtool archive" # Read the libtool library. dlname= library_names= func_source "$file" # Skip this library if it cannot be dlopened. if test -z "$dlname"; then # Warn if it was a shared library. test -n "$library_names" && \ func_warning "'$file' was not linked with '-export-dynamic'" continue fi func_dirname "$file" "" "." dir=$func_dirname_result if test -f "$dir/$objdir/$dlname"; then func_append dir "/$objdir" else if test ! -f "$dir/$dlname"; then func_fatal_error "cannot find '$dlname' in '$dir' or '$dir/$objdir'" fi fi ;; *.lo) # Just add the directory containing the .lo file. func_dirname "$file" "" "." dir=$func_dirname_result ;; *) func_warning "'-dlopen' is ignored for non-libtool libraries and objects" continue ;; esac # Get the absolute pathname. absdir=`cd "$dir" && pwd` test -n "$absdir" && dir=$absdir # Now add the directory to shlibpath_var. if eval "test -z \"\$$shlibpath_var\""; then eval "$shlibpath_var=\"\$dir\"" else eval "$shlibpath_var=\"\$dir:\$$shlibpath_var\"" fi done # This variable tells wrapper scripts just to set shlibpath_var # rather than running their programs. libtool_execute_magic=$magic # Check if any of the arguments is a wrapper script. args= for file do case $file in -* | *.la | *.lo ) ;; *) # Do a test to see if this is really a libtool program. if func_ltwrapper_script_p "$file"; then func_source "$file" # Transform arg to wrapped name. file=$progdir/$program elif func_ltwrapper_executable_p "$file"; then func_ltwrapper_scriptname "$file" func_source "$func_ltwrapper_scriptname_result" # Transform arg to wrapped name. file=$progdir/$program fi ;; esac # Quote arguments (to preserve shell metacharacters). func_append_quoted args "$file" done if $opt_dry_run; then # Display what would be done. if test -n "$shlibpath_var"; then eval "\$ECHO \"\$shlibpath_var=\$$shlibpath_var\"" echo "export $shlibpath_var" fi $ECHO "$cmd$args" exit $EXIT_SUCCESS else if test -n "$shlibpath_var"; then # Export the shlibpath_var. eval "export $shlibpath_var" fi # Restore saved environment variables for lt_var in LANG LANGUAGE LC_ALL LC_CTYPE LC_COLLATE LC_MESSAGES do eval "if test \"\${save_$lt_var+set}\" = set; then $lt_var=\$save_$lt_var; export $lt_var else $lt_unset $lt_var fi" done # Now prepare to actually exec the command. exec_cmd=\$cmd$args fi } test execute = "$opt_mode" && func_mode_execute ${1+"$@"} # func_mode_finish arg... func_mode_finish () { $debug_cmd libs= libdirs= admincmds= for opt in "$nonopt" ${1+"$@"} do if test -d "$opt"; then func_append libdirs " $opt" elif test -f "$opt"; then if func_lalib_unsafe_p "$opt"; then func_append libs " $opt" else func_warning "'$opt' is not a valid libtool archive" fi else func_fatal_error "invalid argument '$opt'" fi done if test -n "$libs"; then if test -n "$lt_sysroot"; then sysroot_regex=`$ECHO "$lt_sysroot" | $SED "$sed_make_literal_regex"` sysroot_cmd="s/\([ ']\)$sysroot_regex/\1/g;" else sysroot_cmd= fi # Remove sysroot references if $opt_dry_run; then for lib in $libs; do echo "removing references to $lt_sysroot and '=' prefixes from $lib" done else tmpdir=`func_mktempdir` for lib in $libs; do $SED -e "$sysroot_cmd s/\([ ']-[LR]\)=/\1/g; s/\([ ']\)=/\1/g" $lib \ > $tmpdir/tmp-la mv -f $tmpdir/tmp-la $lib done ${RM}r "$tmpdir" fi fi if test -n "$finish_cmds$finish_eval" && test -n "$libdirs"; then for libdir in $libdirs; do if test -n "$finish_cmds"; then # Do each command in the finish commands. func_execute_cmds "$finish_cmds" 'admincmds="$admincmds '"$cmd"'"' fi if test -n "$finish_eval"; then # Do the single finish_eval. eval cmds=\"$finish_eval\" $opt_dry_run || eval "$cmds" || func_append admincmds " $cmds" fi done fi # Exit here if they wanted silent mode. $opt_quiet && exit $EXIT_SUCCESS if test -n "$finish_cmds$finish_eval" && test -n "$libdirs"; then echo "----------------------------------------------------------------------" echo "Libraries have been installed in:" for libdir in $libdirs; do $ECHO " $libdir" done echo echo "If you ever happen to want to link against installed libraries" echo "in a given directory, LIBDIR, you must either use libtool, and" echo "specify the full pathname of the library, or use the '-LLIBDIR'" echo "flag during linking and do at least one of the following:" if test -n "$shlibpath_var"; then echo " - add LIBDIR to the '$shlibpath_var' environment variable" echo " during execution" fi if test -n "$runpath_var"; then echo " - add LIBDIR to the '$runpath_var' environment variable" echo " during linking" fi if test -n "$hardcode_libdir_flag_spec"; then libdir=LIBDIR eval flag=\"$hardcode_libdir_flag_spec\" $ECHO " - use the '$flag' linker flag" fi if test -n "$admincmds"; then $ECHO " - have your system administrator run these commands:$admincmds" fi if test -f /etc/ld.so.conf; then echo " - have your system administrator add LIBDIR to '/etc/ld.so.conf'" fi echo echo "See any operating system documentation about shared libraries for" case $host in solaris2.[6789]|solaris2.1[0-9]) echo "more information, such as the ld(1), crle(1) and ld.so(8) manual" echo "pages." ;; *) echo "more information, such as the ld(1) and ld.so(8) manual pages." ;; esac echo "----------------------------------------------------------------------" fi exit $EXIT_SUCCESS } test finish = "$opt_mode" && func_mode_finish ${1+"$@"} # func_mode_install arg... func_mode_install () { $debug_cmd # There may be an optional sh(1) argument at the beginning of # install_prog (especially on Windows NT). if test "$SHELL" = "$nonopt" || test /bin/sh = "$nonopt" || # Allow the use of GNU shtool's install command. case $nonopt in *shtool*) :;; *) false;; esac then # Aesthetically quote it. func_quote_for_eval "$nonopt" install_prog="$func_quote_for_eval_result " arg=$1 shift else install_prog= arg=$nonopt fi # The real first argument should be the name of the installation program. # Aesthetically quote it. func_quote_for_eval "$arg" func_append install_prog "$func_quote_for_eval_result" install_shared_prog=$install_prog case " $install_prog " in *[\\\ /]cp\ *) install_cp=: ;; *) install_cp=false ;; esac # We need to accept at least all the BSD install flags. dest= files= opts= prev= install_type= isdir=false stripme= no_mode=: for arg do arg2= if test -n "$dest"; then func_append files " $dest" dest=$arg continue fi case $arg in -d) isdir=: ;; -f) if $install_cp; then :; else prev=$arg fi ;; -g | -m | -o) prev=$arg ;; -s) stripme=" -s" continue ;; -*) ;; *) # If the previous option needed an argument, then skip it. if test -n "$prev"; then if test X-m = "X$prev" && test -n "$install_override_mode"; then arg2=$install_override_mode no_mode=false fi prev= else dest=$arg continue fi ;; esac # Aesthetically quote the argument. func_quote_for_eval "$arg" func_append install_prog " $func_quote_for_eval_result" if test -n "$arg2"; then func_quote_for_eval "$arg2" fi func_append install_shared_prog " $func_quote_for_eval_result" done test -z "$install_prog" && \ func_fatal_help "you must specify an install program" test -n "$prev" && \ func_fatal_help "the '$prev' option requires an argument" if test -n "$install_override_mode" && $no_mode; then if $install_cp; then :; else func_quote_for_eval "$install_override_mode" func_append install_shared_prog " -m $func_quote_for_eval_result" fi fi if test -z "$files"; then if test -z "$dest"; then func_fatal_help "no file or destination specified" else func_fatal_help "you must specify a destination" fi fi # Strip any trailing slash from the destination. func_stripname '' '/' "$dest" dest=$func_stripname_result # Check to see that the destination is a directory. test -d "$dest" && isdir=: if $isdir; then destdir=$dest destname= else func_dirname_and_basename "$dest" "" "." destdir=$func_dirname_result destname=$func_basename_result # Not a directory, so check to see that there is only one file specified. set dummy $files; shift test "$#" -gt 1 && \ func_fatal_help "'$dest' is not a directory" fi case $destdir in [\\/]* | [A-Za-z]:[\\/]*) ;; *) for file in $files; do case $file in *.lo) ;; *) func_fatal_help "'$destdir' must be an absolute directory name" ;; esac done ;; esac # This variable tells wrapper scripts just to set variables rather # than running their programs. libtool_install_magic=$magic staticlibs= future_libdirs= current_libdirs= for file in $files; do # Do each installation. case $file in *.$libext) # Do the static libraries later. func_append staticlibs " $file" ;; *.la) func_resolve_sysroot "$file" file=$func_resolve_sysroot_result # Check to see that this really is a libtool archive. func_lalib_unsafe_p "$file" \ || func_fatal_help "'$file' is not a valid libtool archive" library_names= old_library= relink_command= func_source "$file" # Add the libdir to current_libdirs if it is the destination. if test "X$destdir" = "X$libdir"; then case "$current_libdirs " in *" $libdir "*) ;; *) func_append current_libdirs " $libdir" ;; esac else # Note the libdir as a future libdir. case "$future_libdirs " in *" $libdir "*) ;; *) func_append future_libdirs " $libdir" ;; esac fi func_dirname "$file" "/" "" dir=$func_dirname_result func_append dir "$objdir" if test -n "$relink_command"; then # Determine the prefix the user has applied to our future dir. inst_prefix_dir=`$ECHO "$destdir" | $SED -e "s%$libdir\$%%"` # Don't allow the user to place us outside of our expected # location b/c this prevents finding dependent libraries that # are installed to the same prefix. # At present, this check doesn't affect windows .dll's that # are installed into $libdir/../bin (currently, that works fine) # but it's something to keep an eye on. test "$inst_prefix_dir" = "$destdir" && \ func_fatal_error "error: cannot install '$file' to a directory not ending in $libdir" if test -n "$inst_prefix_dir"; then # Stick the inst_prefix_dir data into the link command. relink_command=`$ECHO "$relink_command" | $SED "s%@inst_prefix_dir@%-inst-prefix-dir $inst_prefix_dir%"` else relink_command=`$ECHO "$relink_command" | $SED "s%@inst_prefix_dir@%%"` fi func_warning "relinking '$file'" func_show_eval "$relink_command" \ 'func_fatal_error "error: relink '\''$file'\'' with the above command before installing it"' fi # See the names of the shared library. set dummy $library_names; shift if test -n "$1"; then realname=$1 shift srcname=$realname test -n "$relink_command" && srcname=${realname}T # Install the shared library and build the symlinks. func_show_eval "$install_shared_prog $dir/$srcname $destdir/$realname" \ 'exit $?' tstripme=$stripme case $host_os in cygwin* | mingw* | pw32* | cegcc*) case $realname in *.dll.a) tstripme= ;; esac ;; os2*) case $realname in *_dll.a) tstripme= ;; esac ;; esac if test -n "$tstripme" && test -n "$striplib"; then func_show_eval "$striplib $destdir/$realname" 'exit $?' fi if test "$#" -gt 0; then # Delete the old symlinks, and create new ones. # Try 'ln -sf' first, because the 'ln' binary might depend on # the symlink we replace! Solaris /bin/ln does not understand -f, # so we also need to try rm && ln -s. for linkname do test "$linkname" != "$realname" \ && func_show_eval "(cd $destdir && { $LN_S -f $realname $linkname || { $RM $linkname && $LN_S $realname $linkname; }; })" done fi # Do each command in the postinstall commands. lib=$destdir/$realname func_execute_cmds "$postinstall_cmds" 'exit $?' fi # Install the pseudo-library for information purposes. func_basename "$file" name=$func_basename_result instname=$dir/${name}i func_show_eval "$install_prog $instname $destdir/$name" 'exit $?' # Maybe install the static library, too. test -n "$old_library" && func_append staticlibs " $dir/$old_library" ;; *.lo) # Install (i.e. copy) a libtool object. # Figure out destination file name, if it wasn't already specified. if test -n "$destname"; then destfile=$destdir/$destname else func_basename "$file" destfile=$func_basename_result destfile=$destdir/$destfile fi # Deduce the name of the destination old-style object file. case $destfile in *.lo) func_lo2o "$destfile" staticdest=$func_lo2o_result ;; *.$objext) staticdest=$destfile destfile= ;; *) func_fatal_help "cannot copy a libtool object to '$destfile'" ;; esac # Install the libtool object if requested. test -n "$destfile" && \ func_show_eval "$install_prog $file $destfile" 'exit $?' # Install the old object if enabled. if test yes = "$build_old_libs"; then # Deduce the name of the old-style object file. func_lo2o "$file" staticobj=$func_lo2o_result func_show_eval "$install_prog \$staticobj \$staticdest" 'exit $?' fi exit $EXIT_SUCCESS ;; *) # Figure out destination file name, if it wasn't already specified. if test -n "$destname"; then destfile=$destdir/$destname else func_basename "$file" destfile=$func_basename_result destfile=$destdir/$destfile fi # If the file is missing, and there is a .exe on the end, strip it # because it is most likely a libtool script we actually want to # install stripped_ext= case $file in *.exe) if test ! -f "$file"; then func_stripname '' '.exe' "$file" file=$func_stripname_result stripped_ext=.exe fi ;; esac # Do a test to see if this is really a libtool program. case $host in *cygwin* | *mingw*) if func_ltwrapper_executable_p "$file"; then func_ltwrapper_scriptname "$file" wrapper=$func_ltwrapper_scriptname_result else func_stripname '' '.exe' "$file" wrapper=$func_stripname_result fi ;; *) wrapper=$file ;; esac if func_ltwrapper_script_p "$wrapper"; then notinst_deplibs= relink_command= func_source "$wrapper" # Check the variables that should have been set. test -z "$generated_by_libtool_version" && \ func_fatal_error "invalid libtool wrapper script '$wrapper'" finalize=: for lib in $notinst_deplibs; do # Check to see that each library is installed. libdir= if test -f "$lib"; then func_source "$lib" fi libfile=$libdir/`$ECHO "$lib" | $SED 's%^.*/%%g'` if test -n "$libdir" && test ! -f "$libfile"; then func_warning "'$lib' has not been installed in '$libdir'" finalize=false fi done relink_command= func_source "$wrapper" outputname= if test no = "$fast_install" && test -n "$relink_command"; then $opt_dry_run || { if $finalize; then tmpdir=`func_mktempdir` func_basename "$file$stripped_ext" file=$func_basename_result outputname=$tmpdir/$file # Replace the output file specification. relink_command=`$ECHO "$relink_command" | $SED 's%@OUTPUT@%'"$outputname"'%g'` $opt_quiet || { func_quote_for_expand "$relink_command" eval "func_echo $func_quote_for_expand_result" } if eval "$relink_command"; then : else func_error "error: relink '$file' with the above command before installing it" $opt_dry_run || ${RM}r "$tmpdir" continue fi file=$outputname else func_warning "cannot relink '$file'" fi } else # Install the binary that we compiled earlier. file=`$ECHO "$file$stripped_ext" | $SED "s%\([^/]*\)$%$objdir/\1%"` fi fi # remove .exe since cygwin /usr/bin/install will append another # one anyway case $install_prog,$host in */usr/bin/install*,*cygwin*) case $file:$destfile in *.exe:*.exe) # this is ok ;; *.exe:*) destfile=$destfile.exe ;; *:*.exe) func_stripname '' '.exe' "$destfile" destfile=$func_stripname_result ;; esac ;; esac func_show_eval "$install_prog\$stripme \$file \$destfile" 'exit $?' $opt_dry_run || if test -n "$outputname"; then ${RM}r "$tmpdir" fi ;; esac done for file in $staticlibs; do func_basename "$file" name=$func_basename_result # Set up the ranlib parameters. oldlib=$destdir/$name func_to_tool_file "$oldlib" func_convert_file_msys_to_w32 tool_oldlib=$func_to_tool_file_result func_show_eval "$install_prog \$file \$oldlib" 'exit $?' if test -n "$stripme" && test -n "$old_striplib"; then func_show_eval "$old_striplib $tool_oldlib" 'exit $?' fi # Do each command in the postinstall commands. func_execute_cmds "$old_postinstall_cmds" 'exit $?' done test -n "$future_libdirs" && \ func_warning "remember to run '$progname --finish$future_libdirs'" if test -n "$current_libdirs"; then # Maybe just do a dry run. $opt_dry_run && current_libdirs=" -n$current_libdirs" exec_cmd='$SHELL "$progpath" $preserve_args --finish$current_libdirs' else exit $EXIT_SUCCESS fi } test install = "$opt_mode" && func_mode_install ${1+"$@"} # func_generate_dlsyms outputname originator pic_p # Extract symbols from dlprefiles and create ${outputname}S.o with # a dlpreopen symbol table. func_generate_dlsyms () { $debug_cmd my_outputname=$1 my_originator=$2 my_pic_p=${3-false} my_prefix=`$ECHO "$my_originator" | $SED 's%[^a-zA-Z0-9]%_%g'` my_dlsyms= if test -n "$dlfiles$dlprefiles" || test no != "$dlself"; then if test -n "$NM" && test -n "$global_symbol_pipe"; then my_dlsyms=${my_outputname}S.c else func_error "not configured to extract global symbols from dlpreopened files" fi fi if test -n "$my_dlsyms"; then case $my_dlsyms in "") ;; *.c) # Discover the nlist of each of the dlfiles. nlist=$output_objdir/$my_outputname.nm func_show_eval "$RM $nlist ${nlist}S ${nlist}T" # Parse the name list into a source file. func_verbose "creating $output_objdir/$my_dlsyms" $opt_dry_run || $ECHO > "$output_objdir/$my_dlsyms" "\ /* $my_dlsyms - symbol resolution table for '$my_outputname' dlsym emulation. */ /* Generated by $PROGRAM (GNU $PACKAGE) $VERSION */ #ifdef __cplusplus extern \"C\" { #endif #if defined __GNUC__ && (((__GNUC__ == 4) && (__GNUC_MINOR__ >= 4)) || (__GNUC__ > 4)) #pragma GCC diagnostic ignored \"-Wstrict-prototypes\" #endif /* Keep this code in sync between libtool.m4, ltmain, lt_system.h, and tests. */ #if defined _WIN32 || defined __CYGWIN__ || defined _WIN32_WCE /* DATA imports from DLLs on WIN32 can't be const, because runtime relocations are performed -- see ld's documentation on pseudo-relocs. */ # define LT_DLSYM_CONST #elif defined __osf__ /* This system does not cope well with relocations in const data. */ # define LT_DLSYM_CONST #else # define LT_DLSYM_CONST const #endif #define STREQ(s1, s2) (strcmp ((s1), (s2)) == 0) /* External symbol declarations for the compiler. */\ " if test yes = "$dlself"; then func_verbose "generating symbol list for '$output'" $opt_dry_run || echo ': @PROGRAM@ ' > "$nlist" # Add our own program objects to the symbol list. progfiles=`$ECHO "$objs$old_deplibs" | $SP2NL | $SED "$lo2o" | $NL2SP` for progfile in $progfiles; do func_to_tool_file "$progfile" func_convert_file_msys_to_w32 func_verbose "extracting global C symbols from '$func_to_tool_file_result'" $opt_dry_run || eval "$NM $func_to_tool_file_result | $global_symbol_pipe >> '$nlist'" done if test -n "$exclude_expsyms"; then $opt_dry_run || { eval '$EGREP -v " ($exclude_expsyms)$" "$nlist" > "$nlist"T' eval '$MV "$nlist"T "$nlist"' } fi if test -n "$export_symbols_regex"; then $opt_dry_run || { eval '$EGREP -e "$export_symbols_regex" "$nlist" > "$nlist"T' eval '$MV "$nlist"T "$nlist"' } fi # Prepare the list of exported symbols if test -z "$export_symbols"; then export_symbols=$output_objdir/$outputname.exp $opt_dry_run || { $RM $export_symbols eval "$SED -n -e '/^: @PROGRAM@ $/d' -e 's/^.* \(.*\)$/\1/p' "'< "$nlist" > "$export_symbols"' case $host in *cygwin* | *mingw* | *cegcc* ) eval "echo EXPORTS "'> "$output_objdir/$outputname.def"' eval 'cat "$export_symbols" >> "$output_objdir/$outputname.def"' ;; esac } else $opt_dry_run || { eval "$SED -e 's/\([].[*^$]\)/\\\\\1/g' -e 's/^/ /' -e 's/$/$/'"' < "$export_symbols" > "$output_objdir/$outputname.exp"' eval '$GREP -f "$output_objdir/$outputname.exp" < "$nlist" > "$nlist"T' eval '$MV "$nlist"T "$nlist"' case $host in *cygwin* | *mingw* | *cegcc* ) eval "echo EXPORTS "'> "$output_objdir/$outputname.def"' eval 'cat "$nlist" >> "$output_objdir/$outputname.def"' ;; esac } fi fi for dlprefile in $dlprefiles; do func_verbose "extracting global C symbols from '$dlprefile'" func_basename "$dlprefile" name=$func_basename_result case $host in *cygwin* | *mingw* | *cegcc* ) # if an import library, we need to obtain dlname if func_win32_import_lib_p "$dlprefile"; then func_tr_sh "$dlprefile" eval "curr_lafile=\$libfile_$func_tr_sh_result" dlprefile_dlbasename= if test -n "$curr_lafile" && func_lalib_p "$curr_lafile"; then # Use subshell, to avoid clobbering current variable values dlprefile_dlname=`source "$curr_lafile" && echo "$dlname"` if test -n "$dlprefile_dlname"; then func_basename "$dlprefile_dlname" dlprefile_dlbasename=$func_basename_result else # no lafile. user explicitly requested -dlpreopen <import library>. $sharedlib_from_linklib_cmd "$dlprefile" dlprefile_dlbasename=$sharedlib_from_linklib_result fi fi $opt_dry_run || { if test -n "$dlprefile_dlbasename"; then eval '$ECHO ": $dlprefile_dlbasename" >> "$nlist"' else func_warning "Could not compute DLL name from $name" eval '$ECHO ": $name " >> "$nlist"' fi func_to_tool_file "$dlprefile" func_convert_file_msys_to_w32 eval "$NM \"$func_to_tool_file_result\" 2>/dev/null | $global_symbol_pipe | $SED -e '/I __imp/d' -e 's/I __nm_/D /;s/_nm__//' >> '$nlist'" } else # not an import lib $opt_dry_run || { eval '$ECHO ": $name " >> "$nlist"' func_to_tool_file "$dlprefile" func_convert_file_msys_to_w32 eval "$NM \"$func_to_tool_file_result\" 2>/dev/null | $global_symbol_pipe >> '$nlist'" } fi ;; *) $opt_dry_run || { eval '$ECHO ": $name " >> "$nlist"' func_to_tool_file "$dlprefile" func_convert_file_msys_to_w32 eval "$NM \"$func_to_tool_file_result\" 2>/dev/null | $global_symbol_pipe >> '$nlist'" } ;; esac done $opt_dry_run || { # Make sure we have at least an empty file. test -f "$nlist" || : > "$nlist" if test -n "$exclude_expsyms"; then $EGREP -v " ($exclude_expsyms)$" "$nlist" > "$nlist"T $MV "$nlist"T "$nlist" fi # Try sorting and uniquifying the output. if $GREP -v "^: " < "$nlist" | if sort -k 3 </dev/null >/dev/null 2>&1; then sort -k 3 else sort +2 fi | uniq > "$nlist"S; then : else $GREP -v "^: " < "$nlist" > "$nlist"S fi if test -f "$nlist"S; then eval "$global_symbol_to_cdecl"' < "$nlist"S >> "$output_objdir/$my_dlsyms"' else echo '/* NONE */' >> "$output_objdir/$my_dlsyms" fi func_show_eval '$RM "${nlist}I"' if test -n "$global_symbol_to_import"; then eval "$global_symbol_to_import"' < "$nlist"S > "$nlist"I' fi echo >> "$output_objdir/$my_dlsyms" "\ /* The mapping between symbol names and symbols. */ typedef struct { const char *name; void *address; } lt_dlsymlist; extern LT_DLSYM_CONST lt_dlsymlist lt_${my_prefix}_LTX_preloaded_symbols[];\ " if test -s "$nlist"I; then echo >> "$output_objdir/$my_dlsyms" "\ static void lt_syminit(void) { LT_DLSYM_CONST lt_dlsymlist *symbol = lt_${my_prefix}_LTX_preloaded_symbols; for (; symbol->name; ++symbol) {" $SED 's/.*/ if (STREQ (symbol->name, \"&\")) symbol->address = (void *) \&&;/' < "$nlist"I >> "$output_objdir/$my_dlsyms" echo >> "$output_objdir/$my_dlsyms" "\ } }" fi echo >> "$output_objdir/$my_dlsyms" "\ LT_DLSYM_CONST lt_dlsymlist lt_${my_prefix}_LTX_preloaded_symbols[] = { {\"$my_originator\", (void *) 0}," if test -s "$nlist"I; then echo >> "$output_objdir/$my_dlsyms" "\ {\"@INIT@\", (void *) <_syminit}," fi case $need_lib_prefix in no) eval "$global_symbol_to_c_name_address" < "$nlist" >> "$output_objdir/$my_dlsyms" ;; *) eval "$global_symbol_to_c_name_address_lib_prefix" < "$nlist" >> "$output_objdir/$my_dlsyms" ;; esac echo >> "$output_objdir/$my_dlsyms" "\ {0, (void *) 0} }; /* This works around a problem in FreeBSD linker */ #ifdef FREEBSD_WORKAROUND static const void *lt_preloaded_setup() { return lt_${my_prefix}_LTX_preloaded_symbols; } #endif #ifdef __cplusplus } #endif\ " } # !$opt_dry_run pic_flag_for_symtable= case "$compile_command " in *" -static "*) ;; *) case $host in # compiling the symbol table file with pic_flag works around # a FreeBSD bug that causes programs to crash when -lm is # linked before any other PIC object. But we must not use # pic_flag when linking with -static. The problem exists in # FreeBSD 2.2.6 and is fixed in FreeBSD 3.1. *-*-freebsd2.*|*-*-freebsd3.0*|*-*-freebsdelf3.0*) pic_flag_for_symtable=" $pic_flag -DFREEBSD_WORKAROUND" ;; *-*-hpux*) pic_flag_for_symtable=" $pic_flag" ;; *) $my_pic_p && pic_flag_for_symtable=" $pic_flag" ;; esac ;; esac symtab_cflags= for arg in $LTCFLAGS; do case $arg in -pie | -fpie | -fPIE) ;; *) func_append symtab_cflags " $arg" ;; esac done # Now compile the dynamic symbol file. func_show_eval '(cd $output_objdir && $LTCC$symtab_cflags -c$no_builtin_flag$pic_flag_for_symtable "$my_dlsyms")' 'exit $?' # Clean up the generated files. func_show_eval '$RM "$output_objdir/$my_dlsyms" "$nlist" "${nlist}S" "${nlist}T" "${nlist}I"' # Transform the symbol file into the correct name. symfileobj=$output_objdir/${my_outputname}S.$objext case $host in *cygwin* | *mingw* | *cegcc* ) if test -f "$output_objdir/$my_outputname.def"; then compile_command=`$ECHO "$compile_command" | $SED "s%@SYMFILE@%$output_objdir/$my_outputname.def $symfileobj%"` finalize_command=`$ECHO "$finalize_command" | $SED "s%@SYMFILE@%$output_objdir/$my_outputname.def $symfileobj%"` else compile_command=`$ECHO "$compile_command" | $SED "s%@SYMFILE@%$symfileobj%"` finalize_command=`$ECHO "$finalize_command" | $SED "s%@SYMFILE@%$symfileobj%"` fi ;; *) compile_command=`$ECHO "$compile_command" | $SED "s%@SYMFILE@%$symfileobj%"` finalize_command=`$ECHO "$finalize_command" | $SED "s%@SYMFILE@%$symfileobj%"` ;; esac ;; *) func_fatal_error "unknown suffix for '$my_dlsyms'" ;; esac else # We keep going just in case the user didn't refer to # lt_preloaded_symbols. The linker will fail if global_symbol_pipe # really was required. # Nullify the symbol file. compile_command=`$ECHO "$compile_command" | $SED "s% @SYMFILE@%%"` finalize_command=`$ECHO "$finalize_command" | $SED "s% @SYMFILE@%%"` fi } # func_cygming_gnu_implib_p ARG # This predicate returns with zero status (TRUE) if # ARG is a GNU/binutils-style import library. Returns # with nonzero status (FALSE) otherwise. func_cygming_gnu_implib_p () { $debug_cmd func_to_tool_file "$1" func_convert_file_msys_to_w32 func_cygming_gnu_implib_tmp=`$NM "$func_to_tool_file_result" | eval "$global_symbol_pipe" | $EGREP ' (_head_[A-Za-z0-9_]+_[ad]l*|[A-Za-z0-9_]+_[ad]l*_iname)$'` test -n "$func_cygming_gnu_implib_tmp" } # func_cygming_ms_implib_p ARG # This predicate returns with zero status (TRUE) if # ARG is an MS-style import library. Returns # with nonzero status (FALSE) otherwise. func_cygming_ms_implib_p () { $debug_cmd func_to_tool_file "$1" func_convert_file_msys_to_w32 func_cygming_ms_implib_tmp=`$NM "$func_to_tool_file_result" | eval "$global_symbol_pipe" | $GREP '_NULL_IMPORT_DESCRIPTOR'` test -n "$func_cygming_ms_implib_tmp" } # func_win32_libid arg # return the library type of file 'arg' # # Need a lot of goo to handle *both* DLLs and import libs # Has to be a shell function in order to 'eat' the argument # that is supplied when $file_magic_command is called. # Despite the name, also deal with 64 bit binaries. func_win32_libid () { $debug_cmd win32_libid_type=unknown win32_fileres=`file -L $1 2>/dev/null` case $win32_fileres in *ar\ archive\ import\ library*) # definitely import win32_libid_type="x86 archive import" ;; *ar\ archive*) # could be an import, or static # Keep the egrep pattern in sync with the one in _LT_CHECK_MAGIC_METHOD. if eval $OBJDUMP -f $1 | $SED -e '10q' 2>/dev/null | $EGREP 'file format (pei*-i386(.*architecture: i386)?|pe-arm-wince|pe-x86-64)' >/dev/null; then case $nm_interface in "MS dumpbin") if func_cygming_ms_implib_p "$1" || func_cygming_gnu_implib_p "$1" then win32_nmres=import else win32_nmres= fi ;; *) func_to_tool_file "$1" func_convert_file_msys_to_w32 win32_nmres=`eval $NM -f posix -A \"$func_to_tool_file_result\" | $SED -n -e ' 1,100{ / I /{ s|.*|import| p q } }'` ;; esac case $win32_nmres in import*) win32_libid_type="x86 archive import";; *) win32_libid_type="x86 archive static";; esac fi ;; *DLL*) win32_libid_type="x86 DLL" ;; *executable*) # but shell scripts are "executable" too... case $win32_fileres in *MS\ Windows\ PE\ Intel*) win32_libid_type="x86 DLL" ;; esac ;; esac $ECHO "$win32_libid_type" } # func_cygming_dll_for_implib ARG # # Platform-specific function to extract the # name of the DLL associated with the specified # import library ARG. # Invoked by eval'ing the libtool variable # $sharedlib_from_linklib_cmd # Result is available in the variable # $sharedlib_from_linklib_result func_cygming_dll_for_implib () { $debug_cmd sharedlib_from_linklib_result=`$DLLTOOL --identify-strict --identify "$1"` } # func_cygming_dll_for_implib_fallback_core SECTION_NAME LIBNAMEs # # The is the core of a fallback implementation of a # platform-specific function to extract the name of the # DLL associated with the specified import library LIBNAME. # # SECTION_NAME is either .idata$6 or .idata$7, depending # on the platform and compiler that created the implib. # # Echos the name of the DLL associated with the # specified import library. func_cygming_dll_for_implib_fallback_core () { $debug_cmd match_literal=`$ECHO "$1" | $SED "$sed_make_literal_regex"` $OBJDUMP -s --section "$1" "$2" 2>/dev/null | $SED '/^Contents of section '"$match_literal"':/{ # Place marker at beginning of archive member dllname section s/.*/====MARK====/ p d } # These lines can sometimes be longer than 43 characters, but # are always uninteresting /:[ ]*file format pe[i]\{,1\}-/d /^In archive [^:]*:/d # Ensure marker is printed /^====MARK====/p # Remove all lines with less than 43 characters /^.\{43\}/!d # From remaining lines, remove first 43 characters s/^.\{43\}//' | $SED -n ' # Join marker and all lines until next marker into a single line /^====MARK====/ b para H $ b para b :para x s/\n//g # Remove the marker s/^====MARK====// # Remove trailing dots and whitespace s/[\. \t]*$// # Print /./p' | # we now have a list, one entry per line, of the stringified # contents of the appropriate section of all members of the # archive that possess that section. Heuristic: eliminate # all those that have a first or second character that is # a '.' (that is, objdump's representation of an unprintable # character.) This should work for all archives with less than # 0x302f exports -- but will fail for DLLs whose name actually # begins with a literal '.' or a single character followed by # a '.'. # # Of those that remain, print the first one. $SED -e '/^\./d;/^.\./d;q' } # func_cygming_dll_for_implib_fallback ARG # Platform-specific function to extract the # name of the DLL associated with the specified # import library ARG. # # This fallback implementation is for use when $DLLTOOL # does not support the --identify-strict option. # Invoked by eval'ing the libtool variable # $sharedlib_from_linklib_cmd # Result is available in the variable # $sharedlib_from_linklib_result func_cygming_dll_for_implib_fallback () { $debug_cmd if func_cygming_gnu_implib_p "$1"; then # binutils import library sharedlib_from_linklib_result=`func_cygming_dll_for_implib_fallback_core '.idata$7' "$1"` elif func_cygming_ms_implib_p "$1"; then # ms-generated import library sharedlib_from_linklib_result=`func_cygming_dll_for_implib_fallback_core '.idata$6' "$1"` else # unknown sharedlib_from_linklib_result= fi } # func_extract_an_archive dir oldlib func_extract_an_archive () { $debug_cmd f_ex_an_ar_dir=$1; shift f_ex_an_ar_oldlib=$1 if test yes = "$lock_old_archive_extraction"; then lockfile=$f_ex_an_ar_oldlib.lock until $opt_dry_run || ln "$progpath" "$lockfile" 2>/dev/null; do func_echo "Waiting for $lockfile to be removed" sleep 2 done fi func_show_eval "(cd \$f_ex_an_ar_dir && $AR x \"\$f_ex_an_ar_oldlib\")" \ 'stat=$?; rm -f "$lockfile"; exit $stat' if test yes = "$lock_old_archive_extraction"; then $opt_dry_run || rm -f "$lockfile" fi if ($AR t "$f_ex_an_ar_oldlib" | sort | sort -uc >/dev/null 2>&1); then : else func_fatal_error "object name conflicts in archive: $f_ex_an_ar_dir/$f_ex_an_ar_oldlib" fi } # func_extract_archives gentop oldlib ... func_extract_archives () { $debug_cmd my_gentop=$1; shift my_oldlibs=${1+"$@"} my_oldobjs= my_xlib= my_xabs= my_xdir= for my_xlib in $my_oldlibs; do # Extract the objects. case $my_xlib in [\\/]* | [A-Za-z]:[\\/]*) my_xabs=$my_xlib ;; *) my_xabs=`pwd`"/$my_xlib" ;; esac func_basename "$my_xlib" my_xlib=$func_basename_result my_xlib_u=$my_xlib while :; do case " $extracted_archives " in *" $my_xlib_u "*) func_arith $extracted_serial + 1 extracted_serial=$func_arith_result my_xlib_u=lt$extracted_serial-$my_xlib ;; *) break ;; esac done extracted_archives="$extracted_archives $my_xlib_u" my_xdir=$my_gentop/$my_xlib_u func_mkdir_p "$my_xdir" case $host in *-darwin*) func_verbose "Extracting $my_xabs" # Do not bother doing anything if just a dry run $opt_dry_run || { darwin_orig_dir=`pwd` cd $my_xdir || exit $? darwin_archive=$my_xabs darwin_curdir=`pwd` func_basename "$darwin_archive" darwin_base_archive=$func_basename_result darwin_arches=`$LIPO -info "$darwin_archive" 2>/dev/null | $GREP Architectures 2>/dev/null || true` if test -n "$darwin_arches"; then darwin_arches=`$ECHO "$darwin_arches" | $SED -e 's/.*are://'` darwin_arch= func_verbose "$darwin_base_archive has multiple architectures $darwin_arches" for darwin_arch in $darwin_arches; do func_mkdir_p "unfat-$$/$darwin_base_archive-$darwin_arch" $LIPO -thin $darwin_arch -output "unfat-$$/$darwin_base_archive-$darwin_arch/$darwin_base_archive" "$darwin_archive" cd "unfat-$$/$darwin_base_archive-$darwin_arch" func_extract_an_archive "`pwd`" "$darwin_base_archive" cd "$darwin_curdir" $RM "unfat-$$/$darwin_base_archive-$darwin_arch/$darwin_base_archive" done # $darwin_arches ## Okay now we've a bunch of thin objects, gotta fatten them up :) darwin_filelist=`find unfat-$$ -type f -name \*.o -print -o -name \*.lo -print | $SED -e "$sed_basename" | sort -u` darwin_file= darwin_files= for darwin_file in $darwin_filelist; do darwin_files=`find unfat-$$ -name $darwin_file -print | sort | $NL2SP` $LIPO -create -output "$darwin_file" $darwin_files done # $darwin_filelist $RM -rf unfat-$$ cd "$darwin_orig_dir" else cd $darwin_orig_dir func_extract_an_archive "$my_xdir" "$my_xabs" fi # $darwin_arches } # !$opt_dry_run ;; *) func_extract_an_archive "$my_xdir" "$my_xabs" ;; esac my_oldobjs="$my_oldobjs "`find $my_xdir -name \*.$objext -print -o -name \*.lo -print | sort | $NL2SP` done func_extract_archives_result=$my_oldobjs } # func_emit_wrapper [arg=no] # # Emit a libtool wrapper script on stdout. # Don't directly open a file because we may want to # incorporate the script contents within a cygwin/mingw # wrapper executable. Must ONLY be called from within # func_mode_link because it depends on a number of variables # set therein. # # ARG is the value that the WRAPPER_SCRIPT_BELONGS_IN_OBJDIR # variable will take. If 'yes', then the emitted script # will assume that the directory where it is stored is # the $objdir directory. This is a cygwin/mingw-specific # behavior. func_emit_wrapper () { func_emit_wrapper_arg1=${1-no} $ECHO "\ #! $SHELL # $output - temporary wrapper script for $objdir/$outputname # Generated by $PROGRAM (GNU $PACKAGE) $VERSION # # The $output program cannot be directly executed until all the libtool # libraries that it depends on are installed. # # This wrapper script should never be moved out of the build directory. # If it is, it will not operate correctly. # Sed substitution that helps us do robust quoting. It backslashifies # metacharacters that are still active within double-quoted strings. sed_quote_subst='$sed_quote_subst' # Be Bourne compatible if test -n \"\${ZSH_VERSION+set}\" && (emulate sh) >/dev/null 2>&1; then emulate sh NULLCMD=: # Zsh 3.x and 4.x performs word splitting on \${1+\"\$@\"}, which # is contrary to our usage. Disable this feature. alias -g '\${1+\"\$@\"}'='\"\$@\"' setopt NO_GLOB_SUBST else case \`(set -o) 2>/dev/null\` in *posix*) set -o posix;; esac fi BIN_SH=xpg4; export BIN_SH # for Tru64 DUALCASE=1; export DUALCASE # for MKS sh # The HP-UX ksh and POSIX shell print the target directory to stdout # if CDPATH is set. (unset CDPATH) >/dev/null 2>&1 && unset CDPATH relink_command=\"$relink_command\" # This environment variable determines our operation mode. if test \"\$libtool_install_magic\" = \"$magic\"; then # install mode needs the following variables: generated_by_libtool_version='$macro_version' notinst_deplibs='$notinst_deplibs' else # When we are sourced in execute mode, \$file and \$ECHO are already set. if test \"\$libtool_execute_magic\" != \"$magic\"; then file=\"\$0\"" qECHO=`$ECHO "$ECHO" | $SED "$sed_quote_subst"` $ECHO "\ # A function that is used when there is no print builtin or printf. func_fallback_echo () { eval 'cat <<_LTECHO_EOF \$1 _LTECHO_EOF' } ECHO=\"$qECHO\" fi # Very basic option parsing. These options are (a) specific to # the libtool wrapper, (b) are identical between the wrapper # /script/ and the wrapper /executable/ that is used only on # windows platforms, and (c) all begin with the string "--lt-" # (application programs are unlikely to have options that match # this pattern). # # There are only two supported options: --lt-debug and # --lt-dump-script. There is, deliberately, no --lt-help. # # The first argument to this parsing function should be the # script's $0 value, followed by "$@". lt_option_debug= func_parse_lt_options () { lt_script_arg0=\$0 shift for lt_opt do case \"\$lt_opt\" in --lt-debug) lt_option_debug=1 ;; --lt-dump-script) lt_dump_D=\`\$ECHO \"X\$lt_script_arg0\" | $SED -e 's/^X//' -e 's%/[^/]*$%%'\` test \"X\$lt_dump_D\" = \"X\$lt_script_arg0\" && lt_dump_D=. lt_dump_F=\`\$ECHO \"X\$lt_script_arg0\" | $SED -e 's/^X//' -e 's%^.*/%%'\` cat \"\$lt_dump_D/\$lt_dump_F\" exit 0 ;; --lt-*) \$ECHO \"Unrecognized --lt- option: '\$lt_opt'\" 1>&2 exit 1 ;; esac done # Print the debug banner immediately: if test -n \"\$lt_option_debug\"; then echo \"$outputname:$output:\$LINENO: libtool wrapper (GNU $PACKAGE) $VERSION\" 1>&2 fi } # Used when --lt-debug. Prints its arguments to stdout # (redirection is the responsibility of the caller) func_lt_dump_args () { lt_dump_args_N=1; for lt_arg do \$ECHO \"$outputname:$output:\$LINENO: newargv[\$lt_dump_args_N]: \$lt_arg\" lt_dump_args_N=\`expr \$lt_dump_args_N + 1\` done } # Core function for launching the target application func_exec_program_core () { " case $host in # Backslashes separate directories on plain windows *-*-mingw | *-*-os2* | *-cegcc*) $ECHO "\ if test -n \"\$lt_option_debug\"; then \$ECHO \"$outputname:$output:\$LINENO: newargv[0]: \$progdir\\\\\$program\" 1>&2 func_lt_dump_args \${1+\"\$@\"} 1>&2 fi exec \"\$progdir\\\\\$program\" \${1+\"\$@\"} " ;; *) $ECHO "\ if test -n \"\$lt_option_debug\"; then \$ECHO \"$outputname:$output:\$LINENO: newargv[0]: \$progdir/\$program\" 1>&2 func_lt_dump_args \${1+\"\$@\"} 1>&2 fi exec \"\$progdir/\$program\" \${1+\"\$@\"} " ;; esac $ECHO "\ \$ECHO \"\$0: cannot exec \$program \$*\" 1>&2 exit 1 } # A function to encapsulate launching the target application # Strips options in the --lt-* namespace from \$@ and # launches target application with the remaining arguments. func_exec_program () { case \" \$* \" in *\\ --lt-*) for lt_wr_arg do case \$lt_wr_arg in --lt-*) ;; *) set x \"\$@\" \"\$lt_wr_arg\"; shift;; esac shift done ;; esac func_exec_program_core \${1+\"\$@\"} } # Parse options func_parse_lt_options \"\$0\" \${1+\"\$@\"} # Find the directory that this script lives in. thisdir=\`\$ECHO \"\$file\" | $SED 's%/[^/]*$%%'\` test \"x\$thisdir\" = \"x\$file\" && thisdir=. # Follow symbolic links until we get to the real thisdir. file=\`ls -ld \"\$file\" | $SED -n 's/.*-> //p'\` while test -n \"\$file\"; do destdir=\`\$ECHO \"\$file\" | $SED 's%/[^/]*\$%%'\` # If there was a directory component, then change thisdir. if test \"x\$destdir\" != \"x\$file\"; then case \"\$destdir\" in [\\\\/]* | [A-Za-z]:[\\\\/]*) thisdir=\"\$destdir\" ;; *) thisdir=\"\$thisdir/\$destdir\" ;; esac fi file=\`\$ECHO \"\$file\" | $SED 's%^.*/%%'\` file=\`ls -ld \"\$thisdir/\$file\" | $SED -n 's/.*-> //p'\` done # Usually 'no', except on cygwin/mingw when embedded into # the cwrapper. WRAPPER_SCRIPT_BELONGS_IN_OBJDIR=$func_emit_wrapper_arg1 if test \"\$WRAPPER_SCRIPT_BELONGS_IN_OBJDIR\" = \"yes\"; then # special case for '.' if test \"\$thisdir\" = \".\"; then thisdir=\`pwd\` fi # remove .libs from thisdir case \"\$thisdir\" in *[\\\\/]$objdir ) thisdir=\`\$ECHO \"\$thisdir\" | $SED 's%[\\\\/][^\\\\/]*$%%'\` ;; $objdir ) thisdir=. ;; esac fi # Try to get the absolute directory name. absdir=\`cd \"\$thisdir\" && pwd\` test -n \"\$absdir\" && thisdir=\"\$absdir\" " if test yes = "$fast_install"; then $ECHO "\ program=lt-'$outputname'$exeext progdir=\"\$thisdir/$objdir\" if test ! -f \"\$progdir/\$program\" || { file=\`ls -1dt \"\$progdir/\$program\" \"\$progdir/../\$program\" 2>/dev/null | $SED 1q\`; \\ test \"X\$file\" != \"X\$progdir/\$program\"; }; then file=\"\$\$-\$program\" if test ! -d \"\$progdir\"; then $MKDIR \"\$progdir\" else $RM \"\$progdir/\$file\" fi" $ECHO "\ # relink executable if necessary if test -n \"\$relink_command\"; then if relink_command_output=\`eval \$relink_command 2>&1\`; then : else \$ECHO \"\$relink_command_output\" >&2 $RM \"\$progdir/\$file\" exit 1 fi fi $MV \"\$progdir/\$file\" \"\$progdir/\$program\" 2>/dev/null || { $RM \"\$progdir/\$program\"; $MV \"\$progdir/\$file\" \"\$progdir/\$program\"; } $RM \"\$progdir/\$file\" fi" else $ECHO "\ program='$outputname' progdir=\"\$thisdir/$objdir\" " fi $ECHO "\ if test -f \"\$progdir/\$program\"; then" # fixup the dll searchpath if we need to. # # Fix the DLL searchpath if we need to. Do this before prepending # to shlibpath, because on Windows, both are PATH and uninstalled # libraries must come first. if test -n "$dllsearchpath"; then $ECHO "\ # Add the dll search path components to the executable PATH PATH=$dllsearchpath:\$PATH " fi # Export our shlibpath_var if we have one. if test yes = "$shlibpath_overrides_runpath" && test -n "$shlibpath_var" && test -n "$temp_rpath"; then $ECHO "\ # Add our own library path to $shlibpath_var $shlibpath_var=\"$temp_rpath\$$shlibpath_var\" # Some systems cannot cope with colon-terminated $shlibpath_var # The second colon is a workaround for a bug in BeOS R4 sed $shlibpath_var=\`\$ECHO \"\$$shlibpath_var\" | $SED 's/::*\$//'\` export $shlibpath_var " fi $ECHO "\ if test \"\$libtool_execute_magic\" != \"$magic\"; then # Run the actual program with our arguments. func_exec_program \${1+\"\$@\"} fi else # The program doesn't exist. \$ECHO \"\$0: error: '\$progdir/\$program' does not exist\" 1>&2 \$ECHO \"This script is just a wrapper for \$program.\" 1>&2 \$ECHO \"See the $PACKAGE documentation for more information.\" 1>&2 exit 1 fi fi\ " } # func_emit_cwrapperexe_src # emit the source code for a wrapper executable on stdout # Must ONLY be called from within func_mode_link because # it depends on a number of variable set therein. func_emit_cwrapperexe_src () { cat <<EOF /* $cwrappersource - temporary wrapper executable for $objdir/$outputname Generated by $PROGRAM (GNU $PACKAGE) $VERSION The $output program cannot be directly executed until all the libtool libraries that it depends on are installed. This wrapper executable should never be moved out of the build directory. If it is, it will not operate correctly. */ EOF cat <<"EOF" #ifdef _MSC_VER # define _CRT_SECURE_NO_DEPRECATE 1 #endif #include <stdio.h> #include <stdlib.h> #ifdef _MSC_VER # include <direct.h> # include <process.h> # include <io.h> #else # include <unistd.h> # include <stdint.h> # ifdef __CYGWIN__ # include <io.h> # endif #endif #include <malloc.h> #include <stdarg.h> #include <assert.h> #include <string.h> #include <ctype.h> #include <errno.h> #include <fcntl.h> #include <sys/stat.h> #define STREQ(s1, s2) (strcmp ((s1), (s2)) == 0) /* declarations of non-ANSI functions */ #if defined __MINGW32__ # ifdef __STRICT_ANSI__ int _putenv (const char *); # endif #elif defined __CYGWIN__ # ifdef __STRICT_ANSI__ char *realpath (const char *, char *); int putenv (char *); int setenv (const char *, const char *, int); # endif /* #elif defined other_platform || defined ... */ #endif /* portability defines, excluding path handling macros */ #if defined _MSC_VER # define setmode _setmode # define stat _stat # define chmod _chmod # define getcwd _getcwd # define putenv _putenv # define S_IXUSR _S_IEXEC #elif defined __MINGW32__ # define setmode _setmode # define stat _stat # define chmod _chmod # define getcwd _getcwd # define putenv _putenv #elif defined __CYGWIN__ # define HAVE_SETENV # define FOPEN_WB "wb" /* #elif defined other platforms ... */ #endif #if defined PATH_MAX # define LT_PATHMAX PATH_MAX #elif defined MAXPATHLEN # define LT_PATHMAX MAXPATHLEN #else # define LT_PATHMAX 1024 #endif #ifndef S_IXOTH # define S_IXOTH 0 #endif #ifndef S_IXGRP # define S_IXGRP 0 #endif /* path handling portability macros */ #ifndef DIR_SEPARATOR # define DIR_SEPARATOR '/' # define PATH_SEPARATOR ':' #endif #if defined _WIN32 || defined __MSDOS__ || defined __DJGPP__ || \ defined __OS2__ # define HAVE_DOS_BASED_FILE_SYSTEM # define FOPEN_WB "wb" # ifndef DIR_SEPARATOR_2 # define DIR_SEPARATOR_2 '\\' # endif # ifndef PATH_SEPARATOR_2 # define PATH_SEPARATOR_2 ';' # endif #endif #ifndef DIR_SEPARATOR_2 # define IS_DIR_SEPARATOR(ch) ((ch) == DIR_SEPARATOR) #else /* DIR_SEPARATOR_2 */ # define IS_DIR_SEPARATOR(ch) \ (((ch) == DIR_SEPARATOR) || ((ch) == DIR_SEPARATOR_2)) #endif /* DIR_SEPARATOR_2 */ #ifndef PATH_SEPARATOR_2 # define IS_PATH_SEPARATOR(ch) ((ch) == PATH_SEPARATOR) #else /* PATH_SEPARATOR_2 */ # define IS_PATH_SEPARATOR(ch) ((ch) == PATH_SEPARATOR_2) #endif /* PATH_SEPARATOR_2 */ #ifndef FOPEN_WB # define FOPEN_WB "w" #endif #ifndef _O_BINARY # define _O_BINARY 0 #endif #define XMALLOC(type, num) ((type *) xmalloc ((num) * sizeof(type))) #define XFREE(stale) do { \ if (stale) { free (stale); stale = 0; } \ } while (0) #if defined LT_DEBUGWRAPPER static int lt_debug = 1; #else static int lt_debug = 0; #endif const char *program_name = "libtool-wrapper"; /* in case xstrdup fails */ void *xmalloc (size_t num); char *xstrdup (const char *string); const char *base_name (const char *name); char *find_executable (const char *wrapper); char *chase_symlinks (const char *pathspec); int make_executable (const char *path); int check_executable (const char *path); char *strendzap (char *str, const char *pat); void lt_debugprintf (const char *file, int line, const char *fmt, ...); void lt_fatal (const char *file, int line, const char *message, ...); static const char *nonnull (const char *s); static const char *nonempty (const char *s); void lt_setenv (const char *name, const char *value); char *lt_extend_str (const char *orig_value, const char *add, int to_end); void lt_update_exe_path (const char *name, const char *value); void lt_update_lib_path (const char *name, const char *value); char **prepare_spawn (char **argv); void lt_dump_script (FILE *f); EOF cat <<EOF #if __GNUC__ < 4 || (__GNUC__ == 4 && __GNUC_MINOR__ < 5) # define externally_visible volatile #else # define externally_visible __attribute__((externally_visible)) volatile #endif externally_visible const char * MAGIC_EXE = "$magic_exe"; const char * LIB_PATH_VARNAME = "$shlibpath_var"; EOF if test yes = "$shlibpath_overrides_runpath" && test -n "$shlibpath_var" && test -n "$temp_rpath"; then func_to_host_path "$temp_rpath" cat <<EOF const char * LIB_PATH_VALUE = "$func_to_host_path_result"; EOF else cat <<"EOF" const char * LIB_PATH_VALUE = ""; EOF fi if test -n "$dllsearchpath"; then func_to_host_path "$dllsearchpath:" cat <<EOF const char * EXE_PATH_VARNAME = "PATH"; const char * EXE_PATH_VALUE = "$func_to_host_path_result"; EOF else cat <<"EOF" const char * EXE_PATH_VARNAME = ""; const char * EXE_PATH_VALUE = ""; EOF fi if test yes = "$fast_install"; then cat <<EOF const char * TARGET_PROGRAM_NAME = "lt-$outputname"; /* hopefully, no .exe */ EOF else cat <<EOF const char * TARGET_PROGRAM_NAME = "$outputname"; /* hopefully, no .exe */ EOF fi cat <<"EOF" #define LTWRAPPER_OPTION_PREFIX "--lt-" static const char *ltwrapper_option_prefix = LTWRAPPER_OPTION_PREFIX; static const char *dumpscript_opt = LTWRAPPER_OPTION_PREFIX "dump-script"; static const char *debug_opt = LTWRAPPER_OPTION_PREFIX "debug"; int main (int argc, char *argv[]) { char **newargz; int newargc; char *tmp_pathspec; char *actual_cwrapper_path; char *actual_cwrapper_name; char *target_name; char *lt_argv_zero; int rval = 127; int i; program_name = (char *) xstrdup (base_name (argv[0])); newargz = XMALLOC (char *, (size_t) argc + 1); /* very simple arg parsing; don't want to rely on getopt * also, copy all non cwrapper options to newargz, except * argz[0], which is handled differently */ newargc=0; for (i = 1; i < argc; i++) { if (STREQ (argv[i], dumpscript_opt)) { EOF case $host in *mingw* | *cygwin* ) # make stdout use "unix" line endings echo " setmode(1,_O_BINARY);" ;; esac cat <<"EOF" lt_dump_script (stdout); return 0; } if (STREQ (argv[i], debug_opt)) { lt_debug = 1; continue; } if (STREQ (argv[i], ltwrapper_option_prefix)) { /* however, if there is an option in the LTWRAPPER_OPTION_PREFIX namespace, but it is not one of the ones we know about and have already dealt with, above (inluding dump-script), then report an error. Otherwise, targets might begin to believe they are allowed to use options in the LTWRAPPER_OPTION_PREFIX namespace. The first time any user complains about this, we'll need to make LTWRAPPER_OPTION_PREFIX a configure-time option or a configure.ac-settable value. */ lt_fatal (__FILE__, __LINE__, "unrecognized %s option: '%s'", ltwrapper_option_prefix, argv[i]); } /* otherwise ... */ newargz[++newargc] = xstrdup (argv[i]); } newargz[++newargc] = NULL; EOF cat <<EOF /* The GNU banner must be the first non-error debug message */ lt_debugprintf (__FILE__, __LINE__, "libtool wrapper (GNU $PACKAGE) $VERSION\n"); EOF cat <<"EOF" lt_debugprintf (__FILE__, __LINE__, "(main) argv[0]: %s\n", argv[0]); lt_debugprintf (__FILE__, __LINE__, "(main) program_name: %s\n", program_name); tmp_pathspec = find_executable (argv[0]); if (tmp_pathspec == NULL) lt_fatal (__FILE__, __LINE__, "couldn't find %s", argv[0]); lt_debugprintf (__FILE__, __LINE__, "(main) found exe (before symlink chase) at: %s\n", tmp_pathspec); actual_cwrapper_path = chase_symlinks (tmp_pathspec); lt_debugprintf (__FILE__, __LINE__, "(main) found exe (after symlink chase) at: %s\n", actual_cwrapper_path); XFREE (tmp_pathspec); actual_cwrapper_name = xstrdup (base_name (actual_cwrapper_path)); strendzap (actual_cwrapper_path, actual_cwrapper_name); /* wrapper name transforms */ strendzap (actual_cwrapper_name, ".exe"); tmp_pathspec = lt_extend_str (actual_cwrapper_name, ".exe", 1); XFREE (actual_cwrapper_name); actual_cwrapper_name = tmp_pathspec; tmp_pathspec = 0; /* target_name transforms -- use actual target program name; might have lt- prefix */ target_name = xstrdup (base_name (TARGET_PROGRAM_NAME)); strendzap (target_name, ".exe"); tmp_pathspec = lt_extend_str (target_name, ".exe", 1); XFREE (target_name); target_name = tmp_pathspec; tmp_pathspec = 0; lt_debugprintf (__FILE__, __LINE__, "(main) libtool target name: %s\n", target_name); EOF cat <<EOF newargz[0] = XMALLOC (char, (strlen (actual_cwrapper_path) + strlen ("$objdir") + 1 + strlen (actual_cwrapper_name) + 1)); strcpy (newargz[0], actual_cwrapper_path); strcat (newargz[0], "$objdir"); strcat (newargz[0], "/"); EOF cat <<"EOF" /* stop here, and copy so we don't have to do this twice */ tmp_pathspec = xstrdup (newargz[0]); /* do NOT want the lt- prefix here, so use actual_cwrapper_name */ strcat (newargz[0], actual_cwrapper_name); /* DO want the lt- prefix here if it exists, so use target_name */ lt_argv_zero = lt_extend_str (tmp_pathspec, target_name, 1); XFREE (tmp_pathspec); tmp_pathspec = NULL; EOF case $host_os in mingw*) cat <<"EOF" { char* p; while ((p = strchr (newargz[0], '\\')) != NULL) { *p = '/'; } while ((p = strchr (lt_argv_zero, '\\')) != NULL) { *p = '/'; } } EOF ;; esac cat <<"EOF" XFREE (target_name); XFREE (actual_cwrapper_path); XFREE (actual_cwrapper_name); lt_setenv ("BIN_SH", "xpg4"); /* for Tru64 */ lt_setenv ("DUALCASE", "1"); /* for MSK sh */ /* Update the DLL searchpath. EXE_PATH_VALUE ($dllsearchpath) must be prepended before (that is, appear after) LIB_PATH_VALUE ($temp_rpath) because on Windows, both *_VARNAMEs are PATH but uninstalled libraries must come first. */ lt_update_exe_path (EXE_PATH_VARNAME, EXE_PATH_VALUE); lt_update_lib_path (LIB_PATH_VARNAME, LIB_PATH_VALUE); lt_debugprintf (__FILE__, __LINE__, "(main) lt_argv_zero: %s\n", nonnull (lt_argv_zero)); for (i = 0; i < newargc; i++) { lt_debugprintf (__FILE__, __LINE__, "(main) newargz[%d]: %s\n", i, nonnull (newargz[i])); } EOF case $host_os in mingw*) cat <<"EOF" /* execv doesn't actually work on mingw as expected on unix */ newargz = prepare_spawn (newargz); rval = (int) _spawnv (_P_WAIT, lt_argv_zero, (const char * const *) newargz); if (rval == -1) { /* failed to start process */ lt_debugprintf (__FILE__, __LINE__, "(main) failed to launch target \"%s\": %s\n", lt_argv_zero, nonnull (strerror (errno))); return 127; } return rval; EOF ;; *) cat <<"EOF" execv (lt_argv_zero, newargz); return rval; /* =127, but avoids unused variable warning */ EOF ;; esac cat <<"EOF" } void * xmalloc (size_t num) { void *p = (void *) malloc (num); if (!p) lt_fatal (__FILE__, __LINE__, "memory exhausted"); return p; } char * xstrdup (const char *string) { return string ? strcpy ((char *) xmalloc (strlen (string) + 1), string) : NULL; } const char * base_name (const char *name) { const char *base; #if defined HAVE_DOS_BASED_FILE_SYSTEM /* Skip over the disk name in MSDOS pathnames. */ if (isalpha ((unsigned char) name[0]) && name[1] == ':') name += 2; #endif for (base = name; *name; name++) if (IS_DIR_SEPARATOR (*name)) base = name + 1; return base; } int check_executable (const char *path) { struct stat st; lt_debugprintf (__FILE__, __LINE__, "(check_executable): %s\n", nonempty (path)); if ((!path) || (!*path)) return 0; if ((stat (path, &st) >= 0) && (st.st_mode & (S_IXUSR | S_IXGRP | S_IXOTH))) return 1; else return 0; } int make_executable (const char *path) { int rval = 0; struct stat st; lt_debugprintf (__FILE__, __LINE__, "(make_executable): %s\n", nonempty (path)); if ((!path) || (!*path)) return 0; if (stat (path, &st) >= 0) { rval = chmod (path, st.st_mode | S_IXOTH | S_IXGRP | S_IXUSR); } return rval; } /* Searches for the full path of the wrapper. Returns newly allocated full path name if found, NULL otherwise Does not chase symlinks, even on platforms that support them. */ char * find_executable (const char *wrapper) { int has_slash = 0; const char *p; const char *p_next; /* static buffer for getcwd */ char tmp[LT_PATHMAX + 1]; size_t tmp_len; char *concat_name; lt_debugprintf (__FILE__, __LINE__, "(find_executable): %s\n", nonempty (wrapper)); if ((wrapper == NULL) || (*wrapper == '\0')) return NULL; /* Absolute path? */ #if defined HAVE_DOS_BASED_FILE_SYSTEM if (isalpha ((unsigned char) wrapper[0]) && wrapper[1] == ':') { concat_name = xstrdup (wrapper); if (check_executable (concat_name)) return concat_name; XFREE (concat_name); } else { #endif if (IS_DIR_SEPARATOR (wrapper[0])) { concat_name = xstrdup (wrapper); if (check_executable (concat_name)) return concat_name; XFREE (concat_name); } #if defined HAVE_DOS_BASED_FILE_SYSTEM } #endif for (p = wrapper; *p; p++) if (*p == '/') { has_slash = 1; break; } if (!has_slash) { /* no slashes; search PATH */ const char *path = getenv ("PATH"); if (path != NULL) { for (p = path; *p; p = p_next) { const char *q; size_t p_len; for (q = p; *q; q++) if (IS_PATH_SEPARATOR (*q)) break; p_len = (size_t) (q - p); p_next = (*q == '\0' ? q : q + 1); if (p_len == 0) { /* empty path: current directory */ if (getcwd (tmp, LT_PATHMAX) == NULL) lt_fatal (__FILE__, __LINE__, "getcwd failed: %s", nonnull (strerror (errno))); tmp_len = strlen (tmp); concat_name = XMALLOC (char, tmp_len + 1 + strlen (wrapper) + 1); memcpy (concat_name, tmp, tmp_len); concat_name[tmp_len] = '/'; strcpy (concat_name + tmp_len + 1, wrapper); } else { concat_name = XMALLOC (char, p_len + 1 + strlen (wrapper) + 1); memcpy (concat_name, p, p_len); concat_name[p_len] = '/'; strcpy (concat_name + p_len + 1, wrapper); } if (check_executable (concat_name)) return concat_name; XFREE (concat_name); } } /* not found in PATH; assume curdir */ } /* Relative path | not found in path: prepend cwd */ if (getcwd (tmp, LT_PATHMAX) == NULL) lt_fatal (__FILE__, __LINE__, "getcwd failed: %s", nonnull (strerror (errno))); tmp_len = strlen (tmp); concat_name = XMALLOC (char, tmp_len + 1 + strlen (wrapper) + 1); memcpy (concat_name, tmp, tmp_len); concat_name[tmp_len] = '/'; strcpy (concat_name + tmp_len + 1, wrapper); if (check_executable (concat_name)) return concat_name; XFREE (concat_name); return NULL; } char * chase_symlinks (const char *pathspec) { #ifndef S_ISLNK return xstrdup (pathspec); #else char buf[LT_PATHMAX]; struct stat s; char *tmp_pathspec = xstrdup (pathspec); char *p; int has_symlinks = 0; while (strlen (tmp_pathspec) && !has_symlinks) { lt_debugprintf (__FILE__, __LINE__, "checking path component for symlinks: %s\n", tmp_pathspec); if (lstat (tmp_pathspec, &s) == 0) { if (S_ISLNK (s.st_mode) != 0) { has_symlinks = 1; break; } /* search backwards for last DIR_SEPARATOR */ p = tmp_pathspec + strlen (tmp_pathspec) - 1; while ((p > tmp_pathspec) && (!IS_DIR_SEPARATOR (*p))) p--; if ((p == tmp_pathspec) && (!IS_DIR_SEPARATOR (*p))) { /* no more DIR_SEPARATORS left */ break; } *p = '\0'; } else { lt_fatal (__FILE__, __LINE__, "error accessing file \"%s\": %s", tmp_pathspec, nonnull (strerror (errno))); } } XFREE (tmp_pathspec); if (!has_symlinks) { return xstrdup (pathspec); } tmp_pathspec = realpath (pathspec, buf); if (tmp_pathspec == 0) { lt_fatal (__FILE__, __LINE__, "could not follow symlinks for %s", pathspec); } return xstrdup (tmp_pathspec); #endif } char * strendzap (char *str, const char *pat) { size_t len, patlen; assert (str != NULL); assert (pat != NULL); len = strlen (str); patlen = strlen (pat); if (patlen <= len) { str += len - patlen; if (STREQ (str, pat)) *str = '\0'; } return str; } void lt_debugprintf (const char *file, int line, const char *fmt, ...) { va_list args; if (lt_debug) { (void) fprintf (stderr, "%s:%s:%d: ", program_name, file, line); va_start (args, fmt); (void) vfprintf (stderr, fmt, args); va_end (args); } } static void lt_error_core (int exit_status, const char *file, int line, const char *mode, const char *message, va_list ap) { fprintf (stderr, "%s:%s:%d: %s: ", program_name, file, line, mode); vfprintf (stderr, message, ap); fprintf (stderr, ".\n"); if (exit_status >= 0) exit (exit_status); } void lt_fatal (const char *file, int line, const char *message, ...) { va_list ap; va_start (ap, message); lt_error_core (EXIT_FAILURE, file, line, "FATAL", message, ap); va_end (ap); } static const char * nonnull (const char *s) { return s ? s : "(null)"; } static const char * nonempty (const char *s) { return (s && !*s) ? "(empty)" : nonnull (s); } void lt_setenv (const char *name, const char *value) { lt_debugprintf (__FILE__, __LINE__, "(lt_setenv) setting '%s' to '%s'\n", nonnull (name), nonnull (value)); { #ifdef HAVE_SETENV /* always make a copy, for consistency with !HAVE_SETENV */ char *str = xstrdup (value); setenv (name, str, 1); #else size_t len = strlen (name) + 1 + strlen (value) + 1; char *str = XMALLOC (char, len); sprintf (str, "%s=%s", name, value); if (putenv (str) != EXIT_SUCCESS) { XFREE (str); } #endif } } char * lt_extend_str (const char *orig_value, const char *add, int to_end) { char *new_value; if (orig_value && *orig_value) { size_t orig_value_len = strlen (orig_value); size_t add_len = strlen (add); new_value = XMALLOC (char, add_len + orig_value_len + 1); if (to_end) { strcpy (new_value, orig_value); strcpy (new_value + orig_value_len, add); } else { strcpy (new_value, add); strcpy (new_value + add_len, orig_value); } } else { new_value = xstrdup (add); } return new_value; } void lt_update_exe_path (const char *name, const char *value) { lt_debugprintf (__FILE__, __LINE__, "(lt_update_exe_path) modifying '%s' by prepending '%s'\n", nonnull (name), nonnull (value)); if (name && *name && value && *value) { char *new_value = lt_extend_str (getenv (name), value, 0); /* some systems can't cope with a ':'-terminated path #' */ size_t len = strlen (new_value); while ((len > 0) && IS_PATH_SEPARATOR (new_value[len-1])) { new_value[--len] = '\0'; } lt_setenv (name, new_value); XFREE (new_value); } } void lt_update_lib_path (const char *name, const char *value) { lt_debugprintf (__FILE__, __LINE__, "(lt_update_lib_path) modifying '%s' by prepending '%s'\n", nonnull (name), nonnull (value)); if (name && *name && value && *value) { char *new_value = lt_extend_str (getenv (name), value, 0); lt_setenv (name, new_value); XFREE (new_value); } } EOF case $host_os in mingw*) cat <<"EOF" /* Prepares an argument vector before calling spawn(). Note that spawn() does not by itself call the command interpreter (getenv ("COMSPEC") != NULL ? getenv ("COMSPEC") : ({ OSVERSIONINFO v; v.dwOSVersionInfoSize = sizeof(OSVERSIONINFO); GetVersionEx(&v); v.dwPlatformId == VER_PLATFORM_WIN32_NT; }) ? "cmd.exe" : "command.com"). Instead it simply concatenates the arguments, separated by ' ', and calls CreateProcess(). We must quote the arguments since Win32 CreateProcess() interprets characters like ' ', '\t', '\\', '"' (but not '<' and '>') in a special way: - Space and tab are interpreted as delimiters. They are not treated as delimiters if they are surrounded by double quotes: "...". - Unescaped double quotes are removed from the input. Their only effect is that within double quotes, space and tab are treated like normal characters. - Backslashes not followed by double quotes are not special. - But 2*n+1 backslashes followed by a double quote become n backslashes followed by a double quote (n >= 0): \" -> " \\\" -> \" \\\\\" -> \\" */ #define SHELL_SPECIAL_CHARS "\"\\ \001\002\003\004\005\006\007\010\011\012\013\014\015\016\017\020\021\022\023\024\025\026\027\030\031\032\033\034\035\036\037" #define SHELL_SPACE_CHARS " \001\002\003\004\005\006\007\010\011\012\013\014\015\016\017\020\021\022\023\024\025\026\027\030\031\032\033\034\035\036\037" char ** prepare_spawn (char **argv) { size_t argc; char **new_argv; size_t i; /* Count number of arguments. */ for (argc = 0; argv[argc] != NULL; argc++) ; /* Allocate new argument vector. */ new_argv = XMALLOC (char *, argc + 1); /* Put quoted arguments into the new argument vector. */ for (i = 0; i < argc; i++) { const char *string = argv[i]; if (string[0] == '\0') new_argv[i] = xstrdup ("\"\""); else if (strpbrk (string, SHELL_SPECIAL_CHARS) != NULL) { int quote_around = (strpbrk (string, SHELL_SPACE_CHARS) != NULL); size_t length; unsigned int backslashes; const char *s; char *quoted_string; char *p; length = 0; backslashes = 0; if (quote_around) length++; for (s = string; *s != '\0'; s++) { char c = *s; if (c == '"') length += backslashes + 1; length++; if (c == '\\') backslashes++; else backslashes = 0; } if (quote_around) length += backslashes + 1; quoted_string = XMALLOC (char, length + 1); p = quoted_string; backslashes = 0; if (quote_around) *p++ = '"'; for (s = string; *s != '\0'; s++) { char c = *s; if (c == '"') { unsigned int j; for (j = backslashes + 1; j > 0; j--) *p++ = '\\'; } *p++ = c; if (c == '\\') backslashes++; else backslashes = 0; } if (quote_around) { unsigned int j; for (j = backslashes; j > 0; j--) *p++ = '\\'; *p++ = '"'; } *p = '\0'; new_argv[i] = quoted_string; } else new_argv[i] = (char *) string; } new_argv[argc] = NULL; return new_argv; } EOF ;; esac cat <<"EOF" void lt_dump_script (FILE* f) { EOF func_emit_wrapper yes | $SED -n -e ' s/^\(.\{79\}\)\(..*\)/\1\ \2/ h s/\([\\"]\)/\\\1/g s/$/\\n/ s/\([^\n]*\).*/ fputs ("\1", f);/p g D' cat <<"EOF" } EOF } # end: func_emit_cwrapperexe_src # func_win32_import_lib_p ARG # True if ARG is an import lib, as indicated by $file_magic_cmd func_win32_import_lib_p () { $debug_cmd case `eval $file_magic_cmd \"\$1\" 2>/dev/null | $SED -e 10q` in *import*) : ;; *) false ;; esac } # func_suncc_cstd_abi # !!ONLY CALL THIS FOR SUN CC AFTER $compile_command IS FULLY EXPANDED!! # Several compiler flags select an ABI that is incompatible with the # Cstd library. Avoid specifying it if any are in CXXFLAGS. func_suncc_cstd_abi () { $debug_cmd case " $compile_command " in *" -compat=g "*|*\ -std=c++[0-9][0-9]\ *|*" -library=stdcxx4 "*|*" -library=stlport4 "*) suncc_use_cstd_abi=no ;; *) suncc_use_cstd_abi=yes ;; esac } # func_mode_link arg... func_mode_link () { $debug_cmd case $host in *-*-cygwin* | *-*-mingw* | *-*-pw32* | *-*-os2* | *-cegcc*) # It is impossible to link a dll without this setting, and # we shouldn't force the makefile maintainer to figure out # what system we are compiling for in order to pass an extra # flag for every libtool invocation. # allow_undefined=no # FIXME: Unfortunately, there are problems with the above when trying # to make a dll that has undefined symbols, in which case not # even a static library is built. For now, we need to specify # -no-undefined on the libtool link line when we can be certain # that all symbols are satisfied, otherwise we get a static library. allow_undefined=yes ;; *) allow_undefined=yes ;; esac libtool_args=$nonopt base_compile="$nonopt $@" compile_command=$nonopt finalize_command=$nonopt compile_rpath= finalize_rpath= compile_shlibpath= finalize_shlibpath= convenience= old_convenience= deplibs= old_deplibs= compiler_flags= linker_flags= dllsearchpath= lib_search_path=`pwd` inst_prefix_dir= new_inherited_linker_flags= avoid_version=no bindir= dlfiles= dlprefiles= dlself=no export_dynamic=no export_symbols= export_symbols_regex= generated= libobjs= ltlibs= module=no no_install=no objs= os2dllname= non_pic_objects= precious_files_regex= prefer_static_libs=no preload=false prev= prevarg= release= rpath= xrpath= perm_rpath= temp_rpath= thread_safe=no vinfo= vinfo_number=no weak_libs= single_module=$wl-single_module func_infer_tag $base_compile # We need to know -static, to get the right output filenames. for arg do case $arg in -shared) test yes != "$build_libtool_libs" \ && func_fatal_configuration "cannot build a shared library" build_old_libs=no break ;; -all-static | -static | -static-libtool-libs) case $arg in -all-static) if test yes = "$build_libtool_libs" && test -z "$link_static_flag"; then func_warning "complete static linking is impossible in this configuration" fi if test -n "$link_static_flag"; then dlopen_self=$dlopen_self_static fi prefer_static_libs=yes ;; -static) if test -z "$pic_flag" && test -n "$link_static_flag"; then dlopen_self=$dlopen_self_static fi prefer_static_libs=built ;; -static-libtool-libs) if test -z "$pic_flag" && test -n "$link_static_flag"; then dlopen_self=$dlopen_self_static fi prefer_static_libs=yes ;; esac build_libtool_libs=no build_old_libs=yes break ;; esac done # See if our shared archives depend on static archives. test -n "$old_archive_from_new_cmds" && build_old_libs=yes # Go through the arguments, transforming them on the way. while test "$#" -gt 0; do arg=$1 shift func_quote_for_eval "$arg" qarg=$func_quote_for_eval_unquoted_result func_append libtool_args " $func_quote_for_eval_result" # If the previous option needs an argument, assign it. if test -n "$prev"; then case $prev in output) func_append compile_command " @OUTPUT@" func_append finalize_command " @OUTPUT@" ;; esac case $prev in bindir) bindir=$arg prev= continue ;; dlfiles|dlprefiles) $preload || { # Add the symbol object into the linking commands. func_append compile_command " @SYMFILE@" func_append finalize_command " @SYMFILE@" preload=: } case $arg in *.la | *.lo) ;; # We handle these cases below. force) if test no = "$dlself"; then dlself=needless export_dynamic=yes fi prev= continue ;; self) if test dlprefiles = "$prev"; then dlself=yes elif test dlfiles = "$prev" && test yes != "$dlopen_self"; then dlself=yes else dlself=needless export_dynamic=yes fi prev= continue ;; *) if test dlfiles = "$prev"; then func_append dlfiles " $arg" else func_append dlprefiles " $arg" fi prev= continue ;; esac ;; expsyms) export_symbols=$arg test -f "$arg" \ || func_fatal_error "symbol file '$arg' does not exist" prev= continue ;; expsyms_regex) export_symbols_regex=$arg prev= continue ;; framework) case $host in *-*-darwin*) case "$deplibs " in *" $qarg.ltframework "*) ;; *) func_append deplibs " $qarg.ltframework" # this is fixed later ;; esac ;; esac prev= continue ;; inst_prefix) inst_prefix_dir=$arg prev= continue ;; mllvm) # Clang does not use LLVM to link, so we can simply discard any # '-mllvm $arg' options when doing the link step. prev= continue ;; objectlist) if test -f "$arg"; then save_arg=$arg moreargs= for fil in `cat "$save_arg"` do # func_append moreargs " $fil" arg=$fil # A libtool-controlled object. # Check to see that this really is a libtool object. if func_lalib_unsafe_p "$arg"; then pic_object= non_pic_object= # Read the .lo file func_source "$arg" if test -z "$pic_object" || test -z "$non_pic_object" || test none = "$pic_object" && test none = "$non_pic_object"; then func_fatal_error "cannot find name of object for '$arg'" fi # Extract subdirectory from the argument. func_dirname "$arg" "/" "" xdir=$func_dirname_result if test none != "$pic_object"; then # Prepend the subdirectory the object is found in. pic_object=$xdir$pic_object if test dlfiles = "$prev"; then if test yes = "$build_libtool_libs" && test yes = "$dlopen_support"; then func_append dlfiles " $pic_object" prev= continue else # If libtool objects are unsupported, then we need to preload. prev=dlprefiles fi fi # CHECK ME: I think I busted this. -Ossama if test dlprefiles = "$prev"; then # Preload the old-style object. func_append dlprefiles " $pic_object" prev= fi # A PIC object. func_append libobjs " $pic_object" arg=$pic_object fi # Non-PIC object. if test none != "$non_pic_object"; then # Prepend the subdirectory the object is found in. non_pic_object=$xdir$non_pic_object # A standard non-PIC object func_append non_pic_objects " $non_pic_object" if test -z "$pic_object" || test none = "$pic_object"; then arg=$non_pic_object fi else # If the PIC object exists, use it instead. # $xdir was prepended to $pic_object above. non_pic_object=$pic_object func_append non_pic_objects " $non_pic_object" fi else # Only an error if not doing a dry-run. if $opt_dry_run; then # Extract subdirectory from the argument. func_dirname "$arg" "/" "" xdir=$func_dirname_result func_lo2o "$arg" pic_object=$xdir$objdir/$func_lo2o_result non_pic_object=$xdir$func_lo2o_result func_append libobjs " $pic_object" func_append non_pic_objects " $non_pic_object" else func_fatal_error "'$arg' is not a valid libtool object" fi fi done else func_fatal_error "link input file '$arg' does not exist" fi arg=$save_arg prev= continue ;; os2dllname) os2dllname=$arg prev= continue ;; precious_regex) precious_files_regex=$arg prev= continue ;; release) release=-$arg prev= continue ;; rpath | xrpath) # We need an absolute path. case $arg in [\\/]* | [A-Za-z]:[\\/]*) ;; *) func_fatal_error "only absolute run-paths are allowed" ;; esac if test rpath = "$prev"; then case "$rpath " in *" $arg "*) ;; *) func_append rpath " $arg" ;; esac else case "$xrpath " in *" $arg "*) ;; *) func_append xrpath " $arg" ;; esac fi prev= continue ;; shrext) shrext_cmds=$arg prev= continue ;; weak) func_append weak_libs " $arg" prev= continue ;; xcclinker) func_append linker_flags " $qarg" func_append compiler_flags " $qarg" prev= func_append compile_command " $qarg" func_append finalize_command " $qarg" continue ;; xcompiler) func_append compiler_flags " $qarg" prev= func_append compile_command " $qarg" func_append finalize_command " $qarg" continue ;; xlinker) func_append linker_flags " $qarg" func_append compiler_flags " $wl$qarg" prev= func_append compile_command " $wl$qarg" func_append finalize_command " $wl$qarg" continue ;; *) eval "$prev=\"\$arg\"" prev= continue ;; esac fi # test -n "$prev" prevarg=$arg case $arg in -all-static) if test -n "$link_static_flag"; then # See comment for -static flag below, for more details. func_append compile_command " $link_static_flag" func_append finalize_command " $link_static_flag" fi continue ;; -allow-undefined) # FIXME: remove this flag sometime in the future. func_fatal_error "'-allow-undefined' must not be used because it is the default" ;; -avoid-version) avoid_version=yes continue ;; -bindir) prev=bindir continue ;; -dlopen) prev=dlfiles continue ;; -dlpreopen) prev=dlprefiles continue ;; -export-dynamic) export_dynamic=yes continue ;; -export-symbols | -export-symbols-regex) if test -n "$export_symbols" || test -n "$export_symbols_regex"; then func_fatal_error "more than one -exported-symbols argument is not allowed" fi if test X-export-symbols = "X$arg"; then prev=expsyms else prev=expsyms_regex fi continue ;; -framework) prev=framework continue ;; -inst-prefix-dir) prev=inst_prefix continue ;; 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then if test yes = "$build_libtool_libs" && test yes = "$dlopen_support"; then func_append dlfiles " $pic_object" prev= continue else # If libtool objects are unsupported, then we need to preload. prev=dlprefiles fi fi # CHECK ME: I think I busted this. -Ossama if test dlprefiles = "$prev"; then # Preload the old-style object. func_append dlprefiles " $pic_object" prev= fi # A PIC object. func_append libobjs " $pic_object" arg=$pic_object } # Non-PIC object. if test none != "$non_pic_object"; then # Prepend the subdirectory the object is found in. non_pic_object=$xdir$non_pic_object # A standard non-PIC object func_append non_pic_objects " $non_pic_object" if test -z "$pic_object" || test none = "$pic_object"; then arg=$non_pic_object fi else # If the PIC object exists, use it instead. # $xdir was prepended to $pic_object above. non_pic_object=$pic_object func_append non_pic_objects " $non_pic_object" fi else # Only an error if not doing a dry-run. if $opt_dry_run; then # Extract subdirectory from the argument. func_dirname "$arg" "/" "" xdir=$func_dirname_result func_lo2o "$arg" pic_object=$xdir$objdir/$func_lo2o_result non_pic_object=$xdir$func_lo2o_result func_append libobjs " $pic_object" func_append non_pic_objects " $non_pic_object" else func_fatal_error "'$arg' is not a valid libtool object" fi fi ;; 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then eval arg=\"$export_dynamic_flag_spec\" func_append compile_command " $arg" func_append finalize_command " $arg" fi oldlibs= # calculate the name of the file, without its directory func_basename "$output" outputname=$func_basename_result libobjs_save=$libobjs if test -n "$shlibpath_var"; then # get the directories listed in $shlibpath_var eval shlib_search_path=\`\$ECHO \"\$$shlibpath_var\" \| \$SED \'s/:/ /g\'\` else shlib_search_path= fi eval sys_lib_search_path=\"$sys_lib_search_path_spec\" eval sys_lib_dlsearch_path=\"$sys_lib_dlsearch_path_spec\" # Definition is injected by LT_CONFIG during libtool generation. func_munge_path_list sys_lib_dlsearch_path "$LT_SYS_LIBRARY_PATH" func_dirname "$output" "/" "" output_objdir=$func_dirname_result$objdir func_to_tool_file "$output_objdir/" tool_output_objdir=$func_to_tool_file_result # Create the object directory. func_mkdir_p "$output_objdir" # Determine the type of output case $output in "") func_fatal_help "you must specify an output file" ;; 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do case $file in *.la) ;; *) func_fatal_help "libraries can '-dlopen' only libtool libraries: $file" ;; esac done ;; prog) compile_deplibs= finalize_deplibs= alldeplibs=false newdlfiles= newdlprefiles= passes="conv scan dlopen dlpreopen link" ;; *) passes="conv" ;; esac for pass in $passes; do # The preopen pass in lib mode reverses $deplibs; put it back here # so that -L comes before libs that need it for instance... if test lib,link = "$linkmode,$pass"; then ## FIXME: Find the place where the list is rebuilt in the wrong ## order, and fix it there properly tmp_deplibs= for deplib in $deplibs; do tmp_deplibs="$deplib $tmp_deplibs" done deplibs=$tmp_deplibs fi if test lib,link = "$linkmode,$pass" || test prog,scan = "$linkmode,$pass"; then libs=$deplibs deplibs= fi if test prog = "$linkmode"; then case $pass in dlopen) libs=$dlfiles ;; dlpreopen) libs=$dlprefiles ;; link) libs="$deplibs %DEPLIBS% $dependency_libs" ;; esac fi if test lib,dlpreopen = "$linkmode,$pass"; then # Collect and forward deplibs of preopened libtool libs for lib in $dlprefiles; do # Ignore non-libtool-libs dependency_libs= func_resolve_sysroot "$lib" case $lib in *.la) func_source "$func_resolve_sysroot_result" ;; esac # Collect preopened libtool deplibs, except any this library # has declared as weak libs for deplib in $dependency_libs; do func_basename "$deplib" deplib_base=$func_basename_result case " $weak_libs " in *" $deplib_base "*) ;; *) func_append deplibs " $deplib" ;; esac done done libs=$dlprefiles fi if test dlopen = "$pass"; then # Collect dlpreopened libraries save_deplibs=$deplibs deplibs= fi for deplib in $libs; do lib= found=false case $deplib in -mt|-mthreads|-kthread|-Kthread|-pthread|-pthreads|--thread-safe \ |-threads|-fopenmp|-openmp|-mp|-xopenmp|-omp|-qsmp=*) if test prog,link = "$linkmode,$pass"; then compile_deplibs="$deplib $compile_deplibs" finalize_deplibs="$deplib $finalize_deplibs" else func_append compiler_flags " $deplib" if test lib = "$linkmode"; then case "$new_inherited_linker_flags " in *" $deplib "*) ;; * ) func_append new_inherited_linker_flags " $deplib" ;; esac fi fi continue ;; -l*) if test lib != "$linkmode" && test prog != "$linkmode"; then func_warning "'-l' is ignored for archives/objects" continue fi func_stripname '-l' '' "$deplib" name=$func_stripname_result if test lib = "$linkmode"; then searchdirs="$newlib_search_path $lib_search_path $compiler_lib_search_dirs $sys_lib_search_path $shlib_search_path" else searchdirs="$newlib_search_path $lib_search_path $sys_lib_search_path $shlib_search_path" fi for searchdir in $searchdirs; do for search_ext in .la $std_shrext .so .a; do # Search the libtool library lib=$searchdir/lib$name$search_ext if test -f "$lib"; then if test .la = "$search_ext"; then found=: else found=false fi break 2 fi done done if $found; then # deplib is a libtool library # If $allow_libtool_libs_with_static_runtimes && $deplib is a stdlib, # We need to do some special things here, and not later. if test yes = "$allow_libtool_libs_with_static_runtimes"; then case " $predeps $postdeps " in *" $deplib "*) if func_lalib_p "$lib"; then library_names= old_library= func_source "$lib" for l in $old_library $library_names; do ll=$l done if test "X$ll" = "X$old_library"; then # only static version available found=false func_dirname "$lib" "" "." ladir=$func_dirname_result lib=$ladir/$old_library if test prog,link = "$linkmode,$pass"; then compile_deplibs="$deplib $compile_deplibs" finalize_deplibs="$deplib $finalize_deplibs" else deplibs="$deplib $deplibs" test lib = "$linkmode" && newdependency_libs="$deplib $newdependency_libs" fi continue fi fi ;; *) ;; esac fi else # deplib doesn't seem to be a libtool library if test prog,link = "$linkmode,$pass"; then compile_deplibs="$deplib $compile_deplibs" finalize_deplibs="$deplib $finalize_deplibs" else deplibs="$deplib $deplibs" test lib = "$linkmode" && newdependency_libs="$deplib $newdependency_libs" fi continue fi ;; # -l *.ltframework) if test prog,link = "$linkmode,$pass"; then compile_deplibs="$deplib $compile_deplibs" finalize_deplibs="$deplib $finalize_deplibs" else deplibs="$deplib $deplibs" if test lib = "$linkmode"; then case "$new_inherited_linker_flags " in *" $deplib "*) ;; * ) func_append new_inherited_linker_flags " $deplib" ;; esac fi fi continue ;; -L*) case $linkmode in lib) deplibs="$deplib $deplibs" test conv = "$pass" && continue newdependency_libs="$deplib $newdependency_libs" func_stripname '-L' '' "$deplib" func_resolve_sysroot "$func_stripname_result" func_append newlib_search_path " $func_resolve_sysroot_result" ;; prog) if test conv = "$pass"; then deplibs="$deplib $deplibs" continue fi if test scan = "$pass"; then deplibs="$deplib $deplibs" else compile_deplibs="$deplib $compile_deplibs" finalize_deplibs="$deplib $finalize_deplibs" fi func_stripname '-L' '' "$deplib" func_resolve_sysroot "$func_stripname_result" func_append newlib_search_path " $func_resolve_sysroot_result" ;; *) func_warning "'-L' is ignored for archives/objects" ;; esac # linkmode continue ;; # -L -R*) if test link = "$pass"; then func_stripname '-R' '' "$deplib" func_resolve_sysroot "$func_stripname_result" dir=$func_resolve_sysroot_result # Make sure the xrpath contains only unique directories. case "$xrpath " in *" $dir "*) ;; *) func_append xrpath " $dir" ;; esac fi deplibs="$deplib $deplibs" continue ;; *.la) func_resolve_sysroot "$deplib" lib=$func_resolve_sysroot_result ;; *.$libext) if test conv = "$pass"; then deplibs="$deplib $deplibs" continue fi case $linkmode in lib) # Linking convenience modules into shared libraries is allowed, # but linking other static libraries is non-portable. case " $dlpreconveniencelibs " in *" $deplib "*) ;; *) valid_a_lib=false case $deplibs_check_method in match_pattern*) set dummy $deplibs_check_method; shift match_pattern_regex=`expr "$deplibs_check_method" : "$1 \(.*\)"` if eval "\$ECHO \"$deplib\"" 2>/dev/null | $SED 10q \ | $EGREP "$match_pattern_regex" > /dev/null; then valid_a_lib=: fi ;; pass_all) valid_a_lib=: ;; esac if $valid_a_lib; then echo $ECHO "*** Warning: Linking the shared library $output against the" $ECHO "*** static library $deplib is not portable!" deplibs="$deplib $deplibs" else echo $ECHO "*** Warning: Trying to link with static lib archive $deplib." echo "*** I have the capability to make that library automatically link in when" echo "*** you link to this library. But I can only do this if you have a" echo "*** shared version of the library, which you do not appear to have" echo "*** because the file extensions .$libext of this argument makes me believe" echo "*** that it is just a static archive that I should not use here." fi ;; esac continue ;; prog) if test link != "$pass"; then deplibs="$deplib $deplibs" else compile_deplibs="$deplib $compile_deplibs" finalize_deplibs="$deplib $finalize_deplibs" fi continue ;; esac # linkmode ;; # *.$libext *.lo | *.$objext) if test conv = "$pass"; then deplibs="$deplib $deplibs" elif test prog = "$linkmode"; then if test dlpreopen = "$pass" || test yes != "$dlopen_support" || test no = "$build_libtool_libs"; then # If there is no dlopen support or we're linking statically, # we need to preload. func_append newdlprefiles " $deplib" compile_deplibs="$deplib $compile_deplibs" finalize_deplibs="$deplib $finalize_deplibs" else func_append newdlfiles " $deplib" fi fi continue ;; %DEPLIBS%) alldeplibs=: continue ;; esac # case $deplib $found || test -f "$lib" \ || func_fatal_error "cannot find the library '$lib' or unhandled argument '$deplib'" # Check to see that this really is a libtool archive. func_lalib_unsafe_p "$lib" \ || func_fatal_error "'$lib' is not a valid libtool archive" func_dirname "$lib" "" "." ladir=$func_dirname_result dlname= dlopen= dlpreopen= libdir= library_names= old_library= inherited_linker_flags= # If the library was installed with an old release of libtool, # it will not redefine variables installed, or shouldnotlink installed=yes shouldnotlink=no avoidtemprpath= # Read the .la file func_source "$lib" # Convert "-framework foo" to "foo.ltframework" if test -n "$inherited_linker_flags"; then tmp_inherited_linker_flags=`$ECHO "$inherited_linker_flags" | $SED 's/-framework \([^ $]*\)/\1.ltframework/g'` for tmp_inherited_linker_flag in $tmp_inherited_linker_flags; do case " $new_inherited_linker_flags " in *" $tmp_inherited_linker_flag "*) ;; *) func_append new_inherited_linker_flags " $tmp_inherited_linker_flag";; esac done fi dependency_libs=`$ECHO " $dependency_libs" | $SED 's% \([^ $]*\).ltframework% -framework \1%g'` if test lib,link = "$linkmode,$pass" || test prog,scan = "$linkmode,$pass" || { test prog != "$linkmode" && test lib != "$linkmode"; }; then test -n "$dlopen" && func_append dlfiles " $dlopen" test -n "$dlpreopen" && func_append dlprefiles " $dlpreopen" fi if test conv = "$pass"; then # Only check for convenience libraries deplibs="$lib $deplibs" if test -z "$libdir"; then if test -z "$old_library"; then func_fatal_error "cannot find name of link library for '$lib'" fi # It is a libtool convenience library, so add in its objects. func_append convenience " $ladir/$objdir/$old_library" func_append old_convenience " $ladir/$objdir/$old_library" elif test prog != "$linkmode" && test lib != "$linkmode"; then func_fatal_error "'$lib' is not a convenience library" fi tmp_libs= for deplib in $dependency_libs; do deplibs="$deplib $deplibs" if $opt_preserve_dup_deps; then case "$tmp_libs " in *" $deplib "*) func_append specialdeplibs " $deplib" ;; esac fi func_append tmp_libs " $deplib" done continue fi # $pass = conv # Get the name of the library we link against. linklib= if test -n "$old_library" && { test yes = "$prefer_static_libs" || test built,no = "$prefer_static_libs,$installed"; }; then linklib=$old_library else for l in $old_library $library_names; do linklib=$l done fi if test -z "$linklib"; then func_fatal_error "cannot find name of link library for '$lib'" fi # This library was specified with -dlopen. if test dlopen = "$pass"; then test -z "$libdir" \ && func_fatal_error "cannot -dlopen a convenience library: '$lib'" if test -z "$dlname" || test yes != "$dlopen_support" || test no = "$build_libtool_libs" then # If there is no dlname, no dlopen support or we're linking # statically, we need to preload. We also need to preload any # dependent libraries so libltdl's deplib preloader doesn't # bomb out in the load deplibs phase. func_append dlprefiles " $lib $dependency_libs" else func_append newdlfiles " $lib" fi continue fi # $pass = dlopen # We need an absolute path. case $ladir in [\\/]* | [A-Za-z]:[\\/]*) abs_ladir=$ladir ;; *) abs_ladir=`cd "$ladir" && pwd` if test -z "$abs_ladir"; then func_warning "cannot determine absolute directory name of '$ladir'" func_warning "passing it literally to the linker, although it might fail" abs_ladir=$ladir fi ;; esac func_basename "$lib" laname=$func_basename_result # Find the relevant object directory and library name. if test yes = "$installed"; then if test ! -f "$lt_sysroot$libdir/$linklib" && test -f "$abs_ladir/$linklib"; then func_warning "library '$lib' was moved." dir=$ladir absdir=$abs_ladir libdir=$abs_ladir else dir=$lt_sysroot$libdir absdir=$lt_sysroot$libdir fi test yes = "$hardcode_automatic" && avoidtemprpath=yes else if test ! -f "$ladir/$objdir/$linklib" && test -f "$abs_ladir/$linklib"; then dir=$ladir absdir=$abs_ladir # Remove this search path later func_append notinst_path " $abs_ladir" else dir=$ladir/$objdir absdir=$abs_ladir/$objdir # Remove this search path later func_append notinst_path " $abs_ladir" fi fi # $installed = yes func_stripname 'lib' '.la' "$laname" name=$func_stripname_result # This library was specified with -dlpreopen. if test dlpreopen = "$pass"; then if test -z "$libdir" && test prog = "$linkmode"; then func_fatal_error "only libraries may -dlpreopen a convenience library: '$lib'" fi case $host in # special handling for platforms with PE-DLLs. *cygwin* | *mingw* | *cegcc* ) # Linker will automatically link against shared library if both # static and shared are present. Therefore, ensure we extract # symbols from the import library if a shared library is present # (otherwise, the dlopen module name will be incorrect). We do # this by putting the import library name into $newdlprefiles. # We recover the dlopen module name by 'saving' the la file # name in a special purpose variable, and (later) extracting the # dlname from the la file. if test -n "$dlname"; then func_tr_sh "$dir/$linklib" eval "libfile_$func_tr_sh_result=\$abs_ladir/\$laname" func_append newdlprefiles " $dir/$linklib" else func_append newdlprefiles " $dir/$old_library" # Keep a list of preopened convenience libraries to check # that they are being used correctly in the link pass. test -z "$libdir" && \ func_append dlpreconveniencelibs " $dir/$old_library" fi ;; * ) # Prefer using a static library (so that no silly _DYNAMIC symbols # are required to link). if test -n "$old_library"; then func_append newdlprefiles " $dir/$old_library" # Keep a list of preopened convenience libraries to check # that they are being used correctly in the link pass. test -z "$libdir" && \ func_append dlpreconveniencelibs " $dir/$old_library" # Otherwise, use the dlname, so that lt_dlopen finds it. elif test -n "$dlname"; then func_append newdlprefiles " $dir/$dlname" else func_append newdlprefiles " $dir/$linklib" fi ;; esac fi # $pass = dlpreopen if test -z "$libdir"; then # Link the convenience library if test lib = "$linkmode"; then deplibs="$dir/$old_library $deplibs" elif test prog,link = "$linkmode,$pass"; then compile_deplibs="$dir/$old_library $compile_deplibs" finalize_deplibs="$dir/$old_library $finalize_deplibs" else deplibs="$lib $deplibs" # used for prog,scan pass fi continue fi if test prog = "$linkmode" && test link != "$pass"; then func_append newlib_search_path " $ladir" deplibs="$lib $deplibs" linkalldeplibs=false if test no != "$link_all_deplibs" || test -z "$library_names" || test no = "$build_libtool_libs"; then linkalldeplibs=: fi tmp_libs= for deplib in $dependency_libs; do case $deplib in -L*) func_stripname '-L' '' "$deplib" func_resolve_sysroot "$func_stripname_result" func_append newlib_search_path " $func_resolve_sysroot_result" ;; esac # Need to link against all dependency_libs? if $linkalldeplibs; then deplibs="$deplib $deplibs" else # Need to hardcode shared library paths # or/and link against static libraries newdependency_libs="$deplib $newdependency_libs" fi if $opt_preserve_dup_deps; then case "$tmp_libs " in *" $deplib "*) func_append specialdeplibs " $deplib" ;; esac fi func_append tmp_libs " $deplib" done # for deplib continue fi # $linkmode = prog... if test prog,link = "$linkmode,$pass"; then if test -n "$library_names" && { { test no = "$prefer_static_libs" || test built,yes = "$prefer_static_libs,$installed"; } || test -z "$old_library"; }; then # We need to hardcode the library path if test -n "$shlibpath_var" && test -z "$avoidtemprpath"; then # Make sure the rpath contains only unique directories. case $temp_rpath: in *"$absdir:"*) ;; *) func_append temp_rpath "$absdir:" ;; esac fi # Hardcode the library path. # Skip directories that are in the system default run-time # search path. case " $sys_lib_dlsearch_path " in *" $absdir "*) ;; *) case "$compile_rpath " in *" $absdir "*) ;; *) func_append compile_rpath " $absdir" ;; esac ;; esac case " $sys_lib_dlsearch_path " in *" $libdir "*) ;; *) case "$finalize_rpath " in *" $libdir "*) ;; *) func_append finalize_rpath " $libdir" ;; esac ;; esac fi # $linkmode,$pass = prog,link... if $alldeplibs && { test pass_all = "$deplibs_check_method" || { test yes = "$build_libtool_libs" && test -n "$library_names"; }; }; then # We only need to search for static libraries continue fi fi link_static=no # Whether the deplib will be linked statically use_static_libs=$prefer_static_libs if test built = "$use_static_libs" && test yes = "$installed"; then use_static_libs=no fi if test -n "$library_names" && { test no = "$use_static_libs" || test -z "$old_library"; }; then case $host in *cygwin* | *mingw* | *cegcc* | *os2*) # No point in relinking DLLs because paths are not encoded func_append notinst_deplibs " $lib" need_relink=no ;; *) if test no = "$installed"; then func_append notinst_deplibs " $lib" need_relink=yes fi ;; esac # This is a shared library # Warn about portability, can't link against -module's on some # systems (darwin). Don't bleat about dlopened modules though! dlopenmodule= for dlpremoduletest in $dlprefiles; do if test "X$dlpremoduletest" = "X$lib"; then dlopenmodule=$dlpremoduletest break fi done if test -z "$dlopenmodule" && test yes = "$shouldnotlink" && test link = "$pass"; then echo if test prog = "$linkmode"; then $ECHO "*** Warning: Linking the executable $output against the loadable module" else $ECHO "*** Warning: Linking the shared library $output against the loadable module" fi $ECHO "*** $linklib is not portable!" fi if test lib = "$linkmode" && test yes = "$hardcode_into_libs"; then # Hardcode the library path. # Skip directories that are in the system default run-time # search path. case " $sys_lib_dlsearch_path " in *" $absdir "*) ;; *) case "$compile_rpath " in *" $absdir "*) ;; *) func_append compile_rpath " $absdir" ;; esac ;; esac case " $sys_lib_dlsearch_path " in *" $libdir "*) ;; *) case "$finalize_rpath " in *" $libdir "*) ;; *) func_append finalize_rpath " $libdir" ;; esac ;; esac fi if test -n "$old_archive_from_expsyms_cmds"; then # figure out the soname set dummy $library_names shift realname=$1 shift libname=`eval "\\$ECHO \"$libname_spec\""` # use dlname if we got it. it's perfectly good, no? if test -n "$dlname"; then soname=$dlname elif test -n "$soname_spec"; then # bleh windows case $host in *cygwin* | mingw* | *cegcc* | *os2*) func_arith $current - $age major=$func_arith_result versuffix=-$major ;; esac eval soname=\"$soname_spec\" else soname=$realname fi # Make a new name for the extract_expsyms_cmds to use soroot=$soname func_basename "$soroot" soname=$func_basename_result func_stripname 'lib' '.dll' "$soname" newlib=libimp-$func_stripname_result.a # If the library has no export list, then create one now if test -f "$output_objdir/$soname-def"; then : else func_verbose "extracting exported symbol list from '$soname'" func_execute_cmds "$extract_expsyms_cmds" 'exit $?' fi # Create $newlib if test -f "$output_objdir/$newlib"; then :; else func_verbose "generating import library for '$soname'" func_execute_cmds "$old_archive_from_expsyms_cmds" 'exit $?' fi # make sure the library variables are pointing to the new library dir=$output_objdir linklib=$newlib fi # test -n "$old_archive_from_expsyms_cmds" if test prog = "$linkmode" || test relink != "$opt_mode"; then add_shlibpath= add_dir= add= lib_linked=yes case $hardcode_action in immediate | unsupported) if test no = "$hardcode_direct"; then add=$dir/$linklib case $host in *-*-sco3.2v5.0.[024]*) add_dir=-L$dir ;; *-*-sysv4*uw2*) add_dir=-L$dir ;; *-*-sysv5OpenUNIX* | *-*-sysv5UnixWare7.[01].[10]* | \ *-*-unixware7*) add_dir=-L$dir ;; *-*-darwin* ) # if the lib is a (non-dlopened) module then we cannot # link against it, someone is ignoring the earlier warnings if /usr/bin/file -L $add 2> /dev/null | $GREP ": [^:]* bundle" >/dev/null; then if test "X$dlopenmodule" != "X$lib"; then $ECHO "*** Warning: lib $linklib is a module, not a shared library" if test -z "$old_library"; then echo echo "*** And there doesn't seem to be a static archive available" echo "*** The link will probably fail, sorry" else add=$dir/$old_library fi elif test -n "$old_library"; then add=$dir/$old_library fi fi esac elif test no = "$hardcode_minus_L"; then case $host in *-*-sunos*) add_shlibpath=$dir ;; esac add_dir=-L$dir add=-l$name elif test no = "$hardcode_shlibpath_var"; then add_shlibpath=$dir add=-l$name else lib_linked=no fi ;; relink) if test yes = "$hardcode_direct" && test no = "$hardcode_direct_absolute"; then add=$dir/$linklib elif test yes = "$hardcode_minus_L"; then add_dir=-L$absdir # Try looking first in the location we're being installed to. if test -n "$inst_prefix_dir"; then case $libdir in [\\/]*) func_append add_dir " -L$inst_prefix_dir$libdir" ;; esac fi add=-l$name elif test yes = "$hardcode_shlibpath_var"; then add_shlibpath=$dir add=-l$name else lib_linked=no fi ;; *) lib_linked=no ;; esac if test yes != "$lib_linked"; then func_fatal_configuration "unsupported hardcode properties" fi if test -n "$add_shlibpath"; then case :$compile_shlibpath: in *":$add_shlibpath:"*) ;; *) func_append compile_shlibpath "$add_shlibpath:" ;; esac fi if test prog = "$linkmode"; then test -n "$add_dir" && compile_deplibs="$add_dir $compile_deplibs" test -n "$add" && compile_deplibs="$add $compile_deplibs" else test -n "$add_dir" && deplibs="$add_dir $deplibs" test -n "$add" && deplibs="$add $deplibs" if test yes != "$hardcode_direct" && test yes != "$hardcode_minus_L" && test yes = "$hardcode_shlibpath_var"; then case :$finalize_shlibpath: in *":$libdir:"*) ;; *) func_append finalize_shlibpath "$libdir:" ;; esac fi fi fi if test prog = "$linkmode" || test relink = "$opt_mode"; then add_shlibpath= add_dir= add= # Finalize command for both is simple: just hardcode it. if test yes = "$hardcode_direct" && test no = "$hardcode_direct_absolute"; then add=$libdir/$linklib elif test yes = "$hardcode_minus_L"; then add_dir=-L$libdir add=-l$name elif test yes = "$hardcode_shlibpath_var"; then case :$finalize_shlibpath: in *":$libdir:"*) ;; *) func_append finalize_shlibpath "$libdir:" ;; esac add=-l$name elif test yes = "$hardcode_automatic"; then if test -n "$inst_prefix_dir" && test -f "$inst_prefix_dir$libdir/$linklib"; then add=$inst_prefix_dir$libdir/$linklib else add=$libdir/$linklib fi else # We cannot seem to hardcode it, guess we'll fake it. add_dir=-L$libdir # Try looking first in the location we're being installed to. if test -n "$inst_prefix_dir"; then case $libdir in [\\/]*) func_append add_dir " -L$inst_prefix_dir$libdir" ;; esac fi add=-l$name fi if test prog = "$linkmode"; then test -n "$add_dir" && finalize_deplibs="$add_dir $finalize_deplibs" test -n "$add" && finalize_deplibs="$add $finalize_deplibs" else test -n "$add_dir" && deplibs="$add_dir $deplibs" test -n "$add" && deplibs="$add $deplibs" fi fi elif test prog = "$linkmode"; then # Here we assume that one of hardcode_direct or hardcode_minus_L # is not unsupported. This is valid on all known static and # shared platforms. if test unsupported != "$hardcode_direct"; then test -n "$old_library" && linklib=$old_library compile_deplibs="$dir/$linklib $compile_deplibs" finalize_deplibs="$dir/$linklib $finalize_deplibs" else compile_deplibs="-l$name -L$dir $compile_deplibs" finalize_deplibs="-l$name -L$dir $finalize_deplibs" fi elif test yes = "$build_libtool_libs"; then # Not a shared library if test pass_all != "$deplibs_check_method"; then # We're trying link a shared library against a static one # but the system doesn't support it. # Just print a warning and add the library to dependency_libs so # that the program can be linked against the static library. echo $ECHO "*** Warning: This system cannot link to static lib archive $lib." echo "*** I have the capability to make that library automatically link in when" echo "*** you link to this library. But I can only do this if you have a" echo "*** shared version of the library, which you do not appear to have." if test yes = "$module"; then echo "*** But as you try to build a module library, libtool will still create " echo "*** a static module, that should work as long as the dlopening application" echo "*** is linked with the -dlopen flag to resolve symbols at runtime." if test -z "$global_symbol_pipe"; then echo echo "*** However, this would only work if libtool was able to extract symbol" echo "*** lists from a program, using 'nm' or equivalent, but libtool could" echo "*** not find such a program. So, this module is probably useless." echo "*** 'nm' from GNU binutils and a full rebuild may help." fi if test no = "$build_old_libs"; then build_libtool_libs=module build_old_libs=yes else build_libtool_libs=no fi fi else deplibs="$dir/$old_library $deplibs" link_static=yes fi fi # link shared/static library? if test lib = "$linkmode"; then if test -n "$dependency_libs" && { test yes != "$hardcode_into_libs" || test yes = "$build_old_libs" || test yes = "$link_static"; }; then # Extract -R from dependency_libs temp_deplibs= for libdir in $dependency_libs; do case $libdir in -R*) func_stripname '-R' '' "$libdir" temp_xrpath=$func_stripname_result case " $xrpath " in *" $temp_xrpath "*) ;; *) func_append xrpath " $temp_xrpath";; esac;; *) func_append temp_deplibs " $libdir";; esac done dependency_libs=$temp_deplibs fi func_append newlib_search_path " $absdir" # Link against this library test no = "$link_static" && newdependency_libs="$abs_ladir/$laname $newdependency_libs" # ... and its dependency_libs tmp_libs= for deplib in $dependency_libs; do newdependency_libs="$deplib $newdependency_libs" case $deplib in -L*) func_stripname '-L' '' "$deplib" func_resolve_sysroot "$func_stripname_result";; *) func_resolve_sysroot "$deplib" ;; esac if $opt_preserve_dup_deps; then case "$tmp_libs " in *" $func_resolve_sysroot_result "*) func_append specialdeplibs " $func_resolve_sysroot_result" ;; esac fi func_append tmp_libs " $func_resolve_sysroot_result" done if test no != "$link_all_deplibs"; then # Add the search paths of all dependency libraries for deplib in $dependency_libs; do path= case $deplib in -L*) path=$deplib ;; *.la) func_resolve_sysroot "$deplib" deplib=$func_resolve_sysroot_result func_dirname "$deplib" "" "." dir=$func_dirname_result # We need an absolute path. case $dir in [\\/]* | [A-Za-z]:[\\/]*) absdir=$dir ;; *) absdir=`cd "$dir" && pwd` if test -z "$absdir"; then func_warning "cannot determine absolute directory name of '$dir'" absdir=$dir fi ;; esac if $GREP "^installed=no" $deplib > /dev/null; then case $host in *-*-darwin*) depdepl= eval deplibrary_names=`$SED -n -e 's/^library_names=\(.*\)$/\1/p' $deplib` if test -n "$deplibrary_names"; then for tmp in $deplibrary_names; do depdepl=$tmp done if test -f "$absdir/$objdir/$depdepl"; then depdepl=$absdir/$objdir/$depdepl darwin_install_name=`$OTOOL -L $depdepl | awk '{if (NR == 2) {print $1;exit}}'` if test -z "$darwin_install_name"; then darwin_install_name=`$OTOOL64 -L $depdepl | awk '{if (NR == 2) {print $1;exit}}'` fi func_append compiler_flags " $wl-dylib_file $wl$darwin_install_name:$depdepl" func_append linker_flags " -dylib_file $darwin_install_name:$depdepl" path= fi fi ;; *) path=-L$absdir/$objdir ;; esac else eval libdir=`$SED -n -e 's/^libdir=\(.*\)$/\1/p' $deplib` test -z "$libdir" && \ func_fatal_error "'$deplib' is not a valid libtool archive" test "$absdir" != "$libdir" && \ func_warning "'$deplib' seems to be moved" path=-L$absdir fi ;; esac case " $deplibs " in *" $path "*) ;; *) deplibs="$path $deplibs" ;; esac done fi # link_all_deplibs != no fi # linkmode = lib done # for deplib in $libs if test link = "$pass"; then if test prog = "$linkmode"; then compile_deplibs="$new_inherited_linker_flags $compile_deplibs" finalize_deplibs="$new_inherited_linker_flags $finalize_deplibs" else compiler_flags="$compiler_flags "`$ECHO " $new_inherited_linker_flags" | $SED 's% \([^ $]*\).ltframework% -framework \1%g'` fi fi dependency_libs=$newdependency_libs if test dlpreopen = "$pass"; then # Link the dlpreopened libraries before other libraries for deplib in $save_deplibs; do deplibs="$deplib $deplibs" done fi if test dlopen != "$pass"; then test conv = "$pass" || { # Make sure lib_search_path contains only unique directories. lib_search_path= for dir in $newlib_search_path; do case "$lib_search_path " in *" $dir "*) ;; *) func_append lib_search_path " $dir" ;; esac done newlib_search_path= } if test prog,link = "$linkmode,$pass"; then vars="compile_deplibs finalize_deplibs" else vars=deplibs fi for var in $vars dependency_libs; do # Add libraries to $var in reverse order eval tmp_libs=\"\$$var\" new_libs= for deplib in $tmp_libs; do # FIXME: Pedantically, this is the right thing to do, so # that some nasty dependency loop isn't accidentally # broken: #new_libs="$deplib $new_libs" # Pragmatically, this seems to cause very few problems in # practice: case $deplib in -L*) new_libs="$deplib $new_libs" ;; -R*) ;; *) # And here is the reason: when a library appears more # than once as an explicit dependence of a library, or # is implicitly linked in more than once by the # compiler, it is considered special, and multiple # occurrences thereof are not removed. Compare this # with having the same library being listed as a # dependency of multiple other libraries: in this case, # we know (pedantically, we assume) the library does not # need to be listed more than once, so we keep only the # last copy. This is not always right, but it is rare # enough that we require users that really mean to play # such unportable linking tricks to link the library # using -Wl,-lname, so that libtool does not consider it # for duplicate removal. case " $specialdeplibs " in *" $deplib "*) new_libs="$deplib $new_libs" ;; *) case " $new_libs " in *" $deplib "*) ;; *) new_libs="$deplib $new_libs" ;; esac ;; esac ;; esac done tmp_libs= for deplib in $new_libs; do case $deplib in -L*) case " $tmp_libs " in *" $deplib "*) ;; *) func_append tmp_libs " $deplib" ;; esac ;; *) func_append tmp_libs " $deplib" ;; esac done eval $var=\"$tmp_libs\" done # for var fi # Add Sun CC postdeps if required: test CXX = "$tagname" && { case $host_os in linux*) case `$CC -V 2>&1 | sed 5q` in *Sun\ C*) # Sun C++ 5.9 func_suncc_cstd_abi if test no != "$suncc_use_cstd_abi"; then func_append postdeps ' -library=Cstd -library=Crun' fi ;; esac ;; solaris*) func_cc_basename "$CC" case $func_cc_basename_result in CC* | sunCC*) func_suncc_cstd_abi if test no != "$suncc_use_cstd_abi"; then func_append postdeps ' -library=Cstd -library=Crun' fi ;; esac ;; esac } # Last step: remove runtime libs from dependency_libs # (they stay in deplibs) tmp_libs= for i in $dependency_libs; do case " $predeps $postdeps $compiler_lib_search_path " in *" $i "*) i= ;; esac if test -n "$i"; then func_append tmp_libs " $i" fi done dependency_libs=$tmp_libs done # for pass if test prog = "$linkmode"; then dlfiles=$newdlfiles fi if test prog = "$linkmode" || test lib = "$linkmode"; then dlprefiles=$newdlprefiles fi case $linkmode in oldlib) if test -n "$dlfiles$dlprefiles" || test no != "$dlself"; then func_warning "'-dlopen' is ignored for archives" fi case " $deplibs" in *\ -l* | *\ -L*) func_warning "'-l' and '-L' are ignored for archives" ;; esac test -n "$rpath" && \ func_warning "'-rpath' is ignored for archives" test -n "$xrpath" && \ func_warning "'-R' is ignored for archives" test -n "$vinfo" && \ func_warning "'-version-info/-version-number' is ignored for archives" test -n "$release" && \ func_warning "'-release' is ignored for archives" test -n "$export_symbols$export_symbols_regex" && \ func_warning "'-export-symbols' is ignored for archives" # Now set the variables for building old libraries. build_libtool_libs=no oldlibs=$output func_append objs "$old_deplibs" ;; lib) # Make sure we only generate libraries of the form 'libNAME.la'. case $outputname in lib*) func_stripname 'lib' '.la' "$outputname" name=$func_stripname_result eval shared_ext=\"$shrext_cmds\" eval libname=\"$libname_spec\" ;; *) test no = "$module" \ && func_fatal_help "libtool library '$output' must begin with 'lib'" if test no != "$need_lib_prefix"; then # Add the "lib" prefix for modules if required func_stripname '' '.la' "$outputname" name=$func_stripname_result eval shared_ext=\"$shrext_cmds\" eval libname=\"$libname_spec\" else func_stripname '' '.la' "$outputname" libname=$func_stripname_result fi ;; esac if test -n "$objs"; then if test pass_all != "$deplibs_check_method"; then func_fatal_error "cannot build libtool library '$output' from non-libtool objects on this host:$objs" else echo $ECHO "*** Warning: Linking the shared library $output against the non-libtool" $ECHO "*** objects $objs is not portable!" func_append libobjs " $objs" fi fi test no = "$dlself" \ || func_warning "'-dlopen self' is ignored for libtool libraries" set dummy $rpath shift test 1 -lt "$#" \ && func_warning "ignoring multiple '-rpath's for a libtool library" install_libdir=$1 oldlibs= if test -z "$rpath"; then if test yes = "$build_libtool_libs"; then # Building a libtool convenience library. # Some compilers have problems with a '.al' extension so # convenience libraries should have the same extension an # archive normally would. oldlibs="$output_objdir/$libname.$libext $oldlibs" build_libtool_libs=convenience build_old_libs=yes fi test -n "$vinfo" && \ func_warning "'-version-info/-version-number' is ignored for convenience libraries" test -n "$release" && \ func_warning "'-release' is ignored for convenience libraries" else # Parse the version information argument. save_ifs=$IFS; IFS=: set dummy $vinfo 0 0 0 shift IFS=$save_ifs test -n "$7" && \ func_fatal_help "too many parameters to '-version-info'" # convert absolute version numbers to libtool ages # this retains compatibility with .la files and attempts # to make the code below a bit more comprehensible case $vinfo_number in yes) number_major=$1 number_minor=$2 number_revision=$3 # # There are really only two kinds -- those that # use the current revision as the major version # and those that subtract age and use age as # a minor version. But, then there is irix # that has an extra 1 added just for fun # case $version_type in # correct linux to gnu/linux during the next big refactor darwin|freebsd-elf|linux|osf|windows|none) func_arith $number_major + $number_minor current=$func_arith_result age=$number_minor revision=$number_revision ;; freebsd-aout|qnx|sunos) current=$number_major revision=$number_minor age=0 ;; irix|nonstopux) func_arith $number_major + $number_minor current=$func_arith_result age=$number_minor revision=$number_minor lt_irix_increment=no ;; esac ;; no) current=$1 revision=$2 age=$3 ;; esac # Check that each of the things are valid numbers. case $current in 0|[1-9]|[1-9][0-9]|[1-9][0-9][0-9]|[1-9][0-9][0-9][0-9]|[1-9][0-9][0-9][0-9][0-9]) ;; *) func_error "CURRENT '$current' must be a nonnegative integer" func_fatal_error "'$vinfo' is not valid version information" ;; esac case $revision in 0|[1-9]|[1-9][0-9]|[1-9][0-9][0-9]|[1-9][0-9][0-9][0-9]|[1-9][0-9][0-9][0-9][0-9]) ;; *) func_error "REVISION '$revision' must be a nonnegative integer" func_fatal_error "'$vinfo' is not valid version information" ;; esac case $age in 0|[1-9]|[1-9][0-9]|[1-9][0-9][0-9]|[1-9][0-9][0-9][0-9]|[1-9][0-9][0-9][0-9][0-9]) ;; *) func_error "AGE '$age' must be a nonnegative integer" func_fatal_error "'$vinfo' is not valid version information" ;; esac if test "$age" -gt "$current"; then func_error "AGE '$age' is greater than the current interface number '$current'" func_fatal_error "'$vinfo' is not valid version information" fi # Calculate the version variables. major= versuffix= verstring= case $version_type in none) ;; darwin) # Like Linux, but with the current version available in # verstring for coding it into the library header func_arith $current - $age major=.$func_arith_result versuffix=$major.$age.$revision # Darwin ld doesn't like 0 for these options... func_arith $current + 1 minor_current=$func_arith_result xlcverstring="$wl-compatibility_version $wl$minor_current $wl-current_version $wl$minor_current.$revision" verstring="-compatibility_version $minor_current -current_version $minor_current.$revision" # On Darwin other compilers case $CC in nagfor*) verstring="$wl-compatibility_version $wl$minor_current $wl-current_version $wl$minor_current.$revision" ;; *) verstring="-compatibility_version $minor_current -current_version $minor_current.$revision" ;; esac ;; freebsd-aout) major=.$current versuffix=.$current.$revision ;; freebsd-elf) func_arith $current - $age major=.$func_arith_result versuffix=$major.$age.$revision ;; irix | nonstopux) if test no = "$lt_irix_increment"; then func_arith $current - $age else func_arith $current - $age + 1 fi major=$func_arith_result case $version_type in nonstopux) verstring_prefix=nonstopux ;; *) verstring_prefix=sgi ;; esac verstring=$verstring_prefix$major.$revision # Add in all the interfaces that we are compatible with. loop=$revision while test 0 -ne "$loop"; do func_arith $revision - $loop iface=$func_arith_result func_arith $loop - 1 loop=$func_arith_result verstring=$verstring_prefix$major.$iface:$verstring done # Before this point, $major must not contain '.'. major=.$major versuffix=$major.$revision ;; linux) # correct to gnu/linux during the next big refactor func_arith $current - $age major=.$func_arith_result versuffix=$major.$age.$revision ;; osf) func_arith $current - $age major=.$func_arith_result versuffix=.$current.$age.$revision verstring=$current.$age.$revision # Add in all the interfaces that we are compatible with. loop=$age while test 0 -ne "$loop"; do func_arith $current - $loop iface=$func_arith_result func_arith $loop - 1 loop=$func_arith_result verstring=$verstring:$iface.0 done # Make executables depend on our current version. func_append verstring ":$current.0" ;; qnx) major=.$current versuffix=.$current ;; sco) major=.$current versuffix=.$current ;; sunos) major=.$current versuffix=.$current.$revision ;; windows) # Use '-' rather than '.', since we only want one # extension on DOS 8.3 file systems. func_arith $current - $age major=$func_arith_result versuffix=-$major ;; *) func_fatal_configuration "unknown library version type '$version_type'" ;; esac # Clear the version info if we defaulted, and they specified a release. if test -z "$vinfo" && test -n "$release"; then major= case $version_type in darwin) # we can't check for "0.0" in archive_cmds due to quoting # problems, so we reset it completely verstring= ;; *) verstring=0.0 ;; esac if test no = "$need_version"; then versuffix= else versuffix=.0.0 fi fi # Remove version info from name if versioning should be avoided if test yes,no = "$avoid_version,$need_version"; then major= versuffix= verstring= fi # Check to see if the archive will have undefined symbols. if test yes = "$allow_undefined"; then if test unsupported = "$allow_undefined_flag"; then if test yes = "$build_old_libs"; then func_warning "undefined symbols not allowed in $host shared libraries; building static only" build_libtool_libs=no else func_fatal_error "can't build $host shared library unless -no-undefined is specified" fi fi else # Don't allow undefined symbols. allow_undefined_flag=$no_undefined_flag fi fi func_generate_dlsyms "$libname" "$libname" : func_append libobjs " $symfileobj" test " " = "$libobjs" && libobjs= if test relink != "$opt_mode"; then # Remove our outputs, but don't remove object files since they # may have been created when compiling PIC objects. removelist= tempremovelist=`$ECHO "$output_objdir/*"` for p in $tempremovelist; do case $p in *.$objext | *.gcno) ;; $output_objdir/$outputname | $output_objdir/$libname.* | $output_objdir/$libname$release.*) if test -n "$precious_files_regex"; then if $ECHO "$p" | $EGREP -e "$precious_files_regex" >/dev/null 2>&1 then continue fi fi func_append removelist " $p" ;; *) ;; esac done test -n "$removelist" && \ func_show_eval "${RM}r \$removelist" fi # Now set the variables for building old libraries. if test yes = "$build_old_libs" && test convenience != "$build_libtool_libs"; then func_append oldlibs " $output_objdir/$libname.$libext" # Transform .lo files to .o files. oldobjs="$objs "`$ECHO "$libobjs" | $SP2NL | $SED "/\.$libext$/d; $lo2o" | $NL2SP` fi # Eliminate all temporary directories. #for path in $notinst_path; do # lib_search_path=`$ECHO "$lib_search_path " | $SED "s% $path % %g"` # deplibs=`$ECHO "$deplibs " | $SED "s% -L$path % %g"` # dependency_libs=`$ECHO "$dependency_libs " | $SED "s% -L$path % %g"` #done if test -n "$xrpath"; then # If the user specified any rpath flags, then add them. temp_xrpath= for libdir in $xrpath; do func_replace_sysroot "$libdir" func_append temp_xrpath " -R$func_replace_sysroot_result" case "$finalize_rpath " in *" $libdir "*) ;; *) func_append finalize_rpath " $libdir" ;; esac done if test yes != "$hardcode_into_libs" || test yes = "$build_old_libs"; then dependency_libs="$temp_xrpath $dependency_libs" fi fi # Make sure dlfiles contains only unique files that won't be dlpreopened old_dlfiles=$dlfiles dlfiles= for lib in $old_dlfiles; do case " $dlprefiles $dlfiles " in *" $lib "*) ;; *) func_append dlfiles " $lib" ;; esac done # Make sure dlprefiles contains only unique files old_dlprefiles=$dlprefiles dlprefiles= for lib in $old_dlprefiles; do case "$dlprefiles " in *" $lib "*) ;; *) func_append dlprefiles " $lib" ;; esac done if test yes = "$build_libtool_libs"; then if test -n "$rpath"; then case $host in *-*-cygwin* | *-*-mingw* | *-*-pw32* | *-*-os2* | *-*-beos* | *-cegcc* | *-*-haiku*) # these systems don't actually have a c library (as such)! ;; *-*-rhapsody* | *-*-darwin1.[012]) # Rhapsody C library is in the System framework func_append deplibs " System.ltframework" ;; *-*-netbsd*) # Don't link with libc until the a.out ld.so is fixed. ;; *-*-openbsd* | *-*-freebsd* | *-*-dragonfly*) # Do not include libc due to us having libc/libc_r. ;; *-*-sco3.2v5* | *-*-sco5v6*) # Causes problems with __ctype ;; *-*-sysv4.2uw2* | *-*-sysv5* | *-*-unixware* | *-*-OpenUNIX*) # Compiler inserts libc in the correct place for threads to work ;; *) # Add libc to deplibs on all other systems if necessary. if test yes = "$build_libtool_need_lc"; then func_append deplibs " -lc" fi ;; esac fi # Transform deplibs into only deplibs that can be linked in shared. name_save=$name libname_save=$libname release_save=$release versuffix_save=$versuffix major_save=$major # I'm not sure if I'm treating the release correctly. I think # release should show up in the -l (ie -lgmp5) so we don't want to # add it in twice. Is that correct? release= versuffix= major= newdeplibs= droppeddeps=no case $deplibs_check_method in pass_all) # Don't check for shared/static. Everything works. # This might be a little naive. We might want to check # whether the library exists or not. But this is on # osf3 & osf4 and I'm not really sure... Just # implementing what was already the behavior. newdeplibs=$deplibs ;; test_compile) # This code stresses the "libraries are programs" paradigm to its # limits. Maybe even breaks it. We compile a program, linking it # against the deplibs as a proxy for the library. Then we can check # whether they linked in statically or dynamically with ldd. $opt_dry_run || $RM conftest.c cat > conftest.c <<EOF int main() { return 0; } EOF $opt_dry_run || $RM conftest if $LTCC $LTCFLAGS -o conftest conftest.c $deplibs; then ldd_output=`ldd conftest` for i in $deplibs; do case $i in -l*) func_stripname -l '' "$i" name=$func_stripname_result if test yes = "$allow_libtool_libs_with_static_runtimes"; then case " $predeps $postdeps " in *" $i "*) func_append newdeplibs " $i" i= ;; esac fi if test -n "$i"; then libname=`eval "\\$ECHO \"$libname_spec\""` deplib_matches=`eval "\\$ECHO \"$library_names_spec\""` set dummy $deplib_matches; shift deplib_match=$1 if test `expr "$ldd_output" : ".*$deplib_match"` -ne 0; then func_append newdeplibs " $i" else droppeddeps=yes echo $ECHO "*** Warning: dynamic linker does not accept needed library $i." echo "*** I have the capability to make that library automatically link in when" echo "*** you link to this library. But I can only do this if you have a" echo "*** shared version of the library, which I believe you do not have" echo "*** because a test_compile did reveal that the linker did not use it for" echo "*** its dynamic dependency list that programs get resolved with at runtime." fi fi ;; *) func_append newdeplibs " $i" ;; esac done else # Error occurred in the first compile. Let's try to salvage # the situation: Compile a separate program for each library. for i in $deplibs; do case $i in -l*) func_stripname -l '' "$i" name=$func_stripname_result $opt_dry_run || $RM conftest if $LTCC $LTCFLAGS -o conftest conftest.c $i; then ldd_output=`ldd conftest` if test yes = "$allow_libtool_libs_with_static_runtimes"; then case " $predeps $postdeps " in *" $i "*) func_append newdeplibs " $i" i= ;; esac fi if test -n "$i"; then libname=`eval "\\$ECHO \"$libname_spec\""` deplib_matches=`eval "\\$ECHO \"$library_names_spec\""` set dummy $deplib_matches; shift deplib_match=$1 if test `expr "$ldd_output" : ".*$deplib_match"` -ne 0; then func_append newdeplibs " $i" else droppeddeps=yes echo $ECHO "*** Warning: dynamic linker does not accept needed library $i." echo "*** I have the capability to make that library automatically link in when" echo "*** you link to this library. But I can only do this if you have a" echo "*** shared version of the library, which you do not appear to have" echo "*** because a test_compile did reveal that the linker did not use this one" echo "*** as a dynamic dependency that programs can get resolved with at runtime." fi fi else droppeddeps=yes echo $ECHO "*** Warning! Library $i is needed by this library but I was not able to" echo "*** make it link in! You will probably need to install it or some" echo "*** library that it depends on before this library will be fully" echo "*** functional. Installing it before continuing would be even better." fi ;; *) func_append newdeplibs " $i" ;; esac done fi ;; file_magic*) set dummy $deplibs_check_method; shift file_magic_regex=`expr "$deplibs_check_method" : "$1 \(.*\)"` for a_deplib in $deplibs; do case $a_deplib in -l*) func_stripname -l '' "$a_deplib" name=$func_stripname_result if test yes = "$allow_libtool_libs_with_static_runtimes"; then case " $predeps $postdeps " in *" $a_deplib "*) func_append newdeplibs " $a_deplib" a_deplib= ;; esac fi if test -n "$a_deplib"; then libname=`eval "\\$ECHO \"$libname_spec\""` if test -n "$file_magic_glob"; then libnameglob=`func_echo_all "$libname" | $SED -e $file_magic_glob` else libnameglob=$libname fi test yes = "$want_nocaseglob" && nocaseglob=`shopt -p nocaseglob` for i in $lib_search_path $sys_lib_search_path $shlib_search_path; do if test yes = "$want_nocaseglob"; then shopt -s nocaseglob potential_libs=`ls $i/$libnameglob[.-]* 2>/dev/null` $nocaseglob else potential_libs=`ls $i/$libnameglob[.-]* 2>/dev/null` fi for potent_lib in $potential_libs; do # Follow soft links. if ls -lLd "$potent_lib" 2>/dev/null | $GREP " -> " >/dev/null; then continue fi # The statement above tries to avoid entering an # endless loop below, in case of cyclic links. # We might still enter an endless loop, since a link # loop can be closed while we follow links, # but so what? potlib=$potent_lib while test -h "$potlib" 2>/dev/null; do potliblink=`ls -ld $potlib | $SED 's/.* -> //'` case $potliblink in [\\/]* | [A-Za-z]:[\\/]*) potlib=$potliblink;; *) potlib=`$ECHO "$potlib" | $SED 's|[^/]*$||'`"$potliblink";; esac done if eval $file_magic_cmd \"\$potlib\" 2>/dev/null | $SED -e 10q | $EGREP "$file_magic_regex" > /dev/null; then func_append newdeplibs " $a_deplib" a_deplib= break 2 fi done done fi if test -n "$a_deplib"; then droppeddeps=yes echo $ECHO "*** Warning: linker path does not have real file for library $a_deplib." echo "*** I have the capability to make that library automatically link in when" echo "*** you link to this library. But I can only do this if you have a" echo "*** shared version of the library, which you do not appear to have" echo "*** because I did check the linker path looking for a file starting" if test -z "$potlib"; then $ECHO "*** with $libname but no candidates were found. (...for file magic test)" else $ECHO "*** with $libname and none of the candidates passed a file format test" $ECHO "*** using a file magic. Last file checked: $potlib" fi fi ;; *) # Add a -L argument. func_append newdeplibs " $a_deplib" ;; esac done # Gone through all deplibs. ;; match_pattern*) set dummy $deplibs_check_method; shift match_pattern_regex=`expr "$deplibs_check_method" : "$1 \(.*\)"` for a_deplib in $deplibs; do case $a_deplib in -l*) func_stripname -l '' "$a_deplib" name=$func_stripname_result if test yes = "$allow_libtool_libs_with_static_runtimes"; then case " $predeps $postdeps " in *" $a_deplib "*) func_append newdeplibs " $a_deplib" a_deplib= ;; esac fi if test -n "$a_deplib"; then libname=`eval "\\$ECHO \"$libname_spec\""` for i in $lib_search_path $sys_lib_search_path $shlib_search_path; do potential_libs=`ls $i/$libname[.-]* 2>/dev/null` for potent_lib in $potential_libs; do potlib=$potent_lib # see symlink-check above in file_magic test if eval "\$ECHO \"$potent_lib\"" 2>/dev/null | $SED 10q | \ $EGREP "$match_pattern_regex" > /dev/null; then func_append newdeplibs " $a_deplib" a_deplib= break 2 fi done done fi if test -n "$a_deplib"; then droppeddeps=yes echo $ECHO "*** Warning: linker path does not have real file for library $a_deplib." echo "*** I have the capability to make that library automatically link in when" echo "*** you link to this library. But I can only do this if you have a" echo "*** shared version of the library, which you do not appear to have" echo "*** because I did check the linker path looking for a file starting" if test -z "$potlib"; then $ECHO "*** with $libname but no candidates were found. (...for regex pattern test)" else $ECHO "*** with $libname and none of the candidates passed a file format test" $ECHO "*** using a regex pattern. Last file checked: $potlib" fi fi ;; *) # Add a -L argument. func_append newdeplibs " $a_deplib" ;; esac done # Gone through all deplibs. ;; none | unknown | *) newdeplibs= tmp_deplibs=`$ECHO " $deplibs" | $SED 's/ -lc$//; s/ -[LR][^ ]*//g'` if test yes = "$allow_libtool_libs_with_static_runtimes"; then for i in $predeps $postdeps; do # can't use Xsed below, because $i might contain '/' tmp_deplibs=`$ECHO " $tmp_deplibs" | $SED "s|$i||"` done fi case $tmp_deplibs in *[!\ \ ]*) echo if test none = "$deplibs_check_method"; then echo "*** Warning: inter-library dependencies are not supported in this platform." else echo "*** Warning: inter-library dependencies are not known to be supported." fi echo "*** All declared inter-library dependencies are being dropped." droppeddeps=yes ;; esac ;; esac versuffix=$versuffix_save major=$major_save release=$release_save libname=$libname_save name=$name_save case $host in *-*-rhapsody* | *-*-darwin1.[012]) # On Rhapsody replace the C library with the System framework newdeplibs=`$ECHO " $newdeplibs" | $SED 's/ -lc / System.ltframework /'` ;; esac if test yes = "$droppeddeps"; then if test yes = "$module"; then echo echo "*** Warning: libtool could not satisfy all declared inter-library" $ECHO "*** dependencies of module $libname. Therefore, libtool will create" echo "*** a static module, that should work as long as the dlopening" echo "*** application is linked with the -dlopen flag." if test -z "$global_symbol_pipe"; then echo echo "*** However, this would only work if libtool was able to extract symbol" echo "*** lists from a program, using 'nm' or equivalent, but libtool could" echo "*** not find such a program. So, this module is probably useless." echo "*** 'nm' from GNU binutils and a full rebuild may help." fi if test no = "$build_old_libs"; then oldlibs=$output_objdir/$libname.$libext build_libtool_libs=module build_old_libs=yes else build_libtool_libs=no fi else echo "*** The inter-library dependencies that have been dropped here will be" echo "*** automatically added whenever a program is linked with this library" echo "*** or is declared to -dlopen it." if test no = "$allow_undefined"; then echo echo "*** Since this library must not contain undefined symbols," echo "*** because either the platform does not support them or" echo "*** it was explicitly requested with -no-undefined," echo "*** libtool will only create a static version of it." if test no = "$build_old_libs"; then oldlibs=$output_objdir/$libname.$libext build_libtool_libs=module build_old_libs=yes else build_libtool_libs=no fi fi fi fi # Done checking deplibs! deplibs=$newdeplibs fi # Time to change all our "foo.ltframework" stuff back to "-framework foo" case $host in *-*-darwin*) newdeplibs=`$ECHO " $newdeplibs" | $SED 's% \([^ $]*\).ltframework% -framework \1%g'` new_inherited_linker_flags=`$ECHO " $new_inherited_linker_flags" | $SED 's% \([^ $]*\).ltframework% -framework \1%g'` deplibs=`$ECHO " $deplibs" | $SED 's% \([^ $]*\).ltframework% -framework \1%g'` ;; esac # move library search paths that coincide with paths to not yet # installed libraries to the beginning of the library search list new_libs= for path in $notinst_path; do case " $new_libs " in *" -L$path/$objdir "*) ;; *) case " $deplibs " in *" -L$path/$objdir "*) func_append new_libs " -L$path/$objdir" ;; esac ;; esac done for deplib in $deplibs; do case $deplib in -L*) case " $new_libs " in *" $deplib "*) ;; *) func_append new_libs " $deplib" ;; esac ;; *) func_append new_libs " $deplib" ;; esac done deplibs=$new_libs # All the library-specific variables (install_libdir is set above). library_names= old_library= dlname= # Test again, we may have decided not to build it any more if test yes = "$build_libtool_libs"; then # Remove $wl instances when linking with ld. # FIXME: should test the right _cmds variable. case $archive_cmds in *\$LD\ *) wl= ;; esac if test yes = "$hardcode_into_libs"; then # Hardcode the library paths hardcode_libdirs= dep_rpath= rpath=$finalize_rpath test relink = "$opt_mode" || rpath=$compile_rpath$rpath for libdir in $rpath; do if test -n "$hardcode_libdir_flag_spec"; then if test -n "$hardcode_libdir_separator"; then func_replace_sysroot "$libdir" libdir=$func_replace_sysroot_result if test -z "$hardcode_libdirs"; then hardcode_libdirs=$libdir else # Just accumulate the unique libdirs. case $hardcode_libdir_separator$hardcode_libdirs$hardcode_libdir_separator in *"$hardcode_libdir_separator$libdir$hardcode_libdir_separator"*) ;; *) func_append hardcode_libdirs "$hardcode_libdir_separator$libdir" ;; esac fi else eval flag=\"$hardcode_libdir_flag_spec\" func_append dep_rpath " $flag" fi elif test -n "$runpath_var"; then case "$perm_rpath " in *" $libdir "*) ;; *) func_append perm_rpath " $libdir" ;; esac fi done # Substitute the hardcoded libdirs into the rpath. if test -n "$hardcode_libdir_separator" && test -n "$hardcode_libdirs"; then libdir=$hardcode_libdirs eval "dep_rpath=\"$hardcode_libdir_flag_spec\"" fi if test -n "$runpath_var" && test -n "$perm_rpath"; then # We should set the runpath_var. rpath= for dir in $perm_rpath; do func_append rpath "$dir:" done eval "$runpath_var='$rpath\$$runpath_var'; export $runpath_var" fi test -n "$dep_rpath" && deplibs="$dep_rpath $deplibs" fi shlibpath=$finalize_shlibpath test relink = "$opt_mode" || shlibpath=$compile_shlibpath$shlibpath if test -n "$shlibpath"; then eval "$shlibpath_var='$shlibpath\$$shlibpath_var'; export $shlibpath_var" fi # Get the real and link names of the library. eval shared_ext=\"$shrext_cmds\" eval library_names=\"$library_names_spec\" set dummy $library_names shift realname=$1 shift if test -n "$soname_spec"; then eval soname=\"$soname_spec\" else soname=$realname fi if test -z "$dlname"; then dlname=$soname fi lib=$output_objdir/$realname linknames= for link do func_append linknames " $link" done # Use standard objects if they are pic test -z "$pic_flag" && libobjs=`$ECHO "$libobjs" | $SP2NL | $SED "$lo2o" | $NL2SP` test "X$libobjs" = "X " && libobjs= delfiles= if test -n "$export_symbols" && test -n "$include_expsyms"; then $opt_dry_run || cp "$export_symbols" "$output_objdir/$libname.uexp" export_symbols=$output_objdir/$libname.uexp func_append delfiles " $export_symbols" fi orig_export_symbols= case $host_os in cygwin* | mingw* | cegcc*) if test -n "$export_symbols" && test -z "$export_symbols_regex"; then # exporting using user supplied symfile func_dll_def_p "$export_symbols" || { # and it's NOT already a .def file. Must figure out # which of the given symbols are data symbols and tag # them as such. So, trigger use of export_symbols_cmds. # export_symbols gets reassigned inside the "prepare # the list of exported symbols" if statement, so the # include_expsyms logic still works. orig_export_symbols=$export_symbols export_symbols= always_export_symbols=yes } fi ;; esac # Prepare the list of exported symbols if test -z "$export_symbols"; then if test yes = "$always_export_symbols" || test -n "$export_symbols_regex"; then func_verbose "generating symbol list for '$libname.la'" export_symbols=$output_objdir/$libname.exp $opt_dry_run || $RM $export_symbols cmds=$export_symbols_cmds save_ifs=$IFS; IFS='~' for cmd1 in $cmds; do IFS=$save_ifs # Take the normal branch if the nm_file_list_spec branch # doesn't work or if tool conversion is not needed. case $nm_file_list_spec~$to_tool_file_cmd in *~func_convert_file_noop | *~func_convert_file_msys_to_w32 | ~*) try_normal_branch=yes eval cmd=\"$cmd1\" func_len " $cmd" len=$func_len_result ;; *) try_normal_branch=no ;; esac if test yes = "$try_normal_branch" \ && { test "$len" -lt "$max_cmd_len" \ || test "$max_cmd_len" -le -1; } then func_show_eval "$cmd" 'exit $?' skipped_export=false elif test -n "$nm_file_list_spec"; then func_basename "$output" output_la=$func_basename_result save_libobjs=$libobjs save_output=$output output=$output_objdir/$output_la.nm func_to_tool_file "$output" libobjs=$nm_file_list_spec$func_to_tool_file_result func_append delfiles " $output" func_verbose "creating $NM input file list: $output" for obj in $save_libobjs; do func_to_tool_file "$obj" $ECHO "$func_to_tool_file_result" done > "$output" eval cmd=\"$cmd1\" func_show_eval "$cmd" 'exit $?' output=$save_output libobjs=$save_libobjs skipped_export=false else # The command line is too long to execute in one step. func_verbose "using reloadable object file for export list..." skipped_export=: # Break out early, otherwise skipped_export may be # set to false by a later but shorter cmd. break fi done IFS=$save_ifs if test -n "$export_symbols_regex" && test : != "$skipped_export"; then func_show_eval '$EGREP -e "$export_symbols_regex" "$export_symbols" > "${export_symbols}T"' func_show_eval '$MV "${export_symbols}T" "$export_symbols"' fi fi fi if test -n "$export_symbols" && test -n "$include_expsyms"; then tmp_export_symbols=$export_symbols test -n "$orig_export_symbols" && tmp_export_symbols=$orig_export_symbols $opt_dry_run || eval '$ECHO "$include_expsyms" | $SP2NL >> "$tmp_export_symbols"' fi if test : != "$skipped_export" && test -n "$orig_export_symbols"; then # The given exports_symbols file has to be filtered, so filter it. func_verbose "filter symbol list for '$libname.la' to tag DATA exports" # FIXME: $output_objdir/$libname.filter potentially contains lots of # 's' commands, which not all seds can handle. GNU sed should be fine # though. Also, the filter scales superlinearly with the number of # global variables. join(1) would be nice here, but unfortunately # isn't a blessed tool. $opt_dry_run || $SED -e '/[ ,]DATA/!d;s,\(.*\)\([ \,].*\),s|^\1$|\1\2|,' < $export_symbols > $output_objdir/$libname.filter func_append delfiles " $export_symbols $output_objdir/$libname.filter" export_symbols=$output_objdir/$libname.def $opt_dry_run || $SED -f $output_objdir/$libname.filter < $orig_export_symbols > $export_symbols fi tmp_deplibs= for test_deplib in $deplibs; do case " $convenience " in *" $test_deplib "*) ;; *) func_append tmp_deplibs " $test_deplib" ;; esac done deplibs=$tmp_deplibs if test -n "$convenience"; then if test -n "$whole_archive_flag_spec" && test yes = "$compiler_needs_object" && test -z "$libobjs"; then # extract the archives, so we have objects to list. # TODO: could optimize this to just extract one archive. whole_archive_flag_spec= fi if test -n "$whole_archive_flag_spec"; then save_libobjs=$libobjs eval libobjs=\"\$libobjs $whole_archive_flag_spec\" test "X$libobjs" = "X " && libobjs= else gentop=$output_objdir/${outputname}x func_append generated " $gentop" func_extract_archives $gentop $convenience func_append libobjs " $func_extract_archives_result" test "X$libobjs" = "X " && libobjs= fi fi if test yes = "$thread_safe" && test -n "$thread_safe_flag_spec"; then eval flag=\"$thread_safe_flag_spec\" func_append linker_flags " $flag" fi # Make a backup of the uninstalled library when relinking if test relink = "$opt_mode"; then $opt_dry_run || eval '(cd $output_objdir && $RM ${realname}U && $MV $realname ${realname}U)' || exit $? fi # Do each of the archive commands. if test yes = "$module" && test -n "$module_cmds"; then if test -n "$export_symbols" && test -n "$module_expsym_cmds"; then eval test_cmds=\"$module_expsym_cmds\" cmds=$module_expsym_cmds else eval test_cmds=\"$module_cmds\" cmds=$module_cmds fi else if test -n "$export_symbols" && test -n "$archive_expsym_cmds"; then eval test_cmds=\"$archive_expsym_cmds\" cmds=$archive_expsym_cmds else eval test_cmds=\"$archive_cmds\" cmds=$archive_cmds fi fi if test : != "$skipped_export" && func_len " $test_cmds" && len=$func_len_result && test "$len" -lt "$max_cmd_len" || test "$max_cmd_len" -le -1; then : else # The command line is too long to link in one step, link piecewise # or, if using GNU ld and skipped_export is not :, use a linker # script. # Save the value of $output and $libobjs because we want to # use them later. If we have whole_archive_flag_spec, we # want to use save_libobjs as it was before # whole_archive_flag_spec was expanded, because we can't # assume the linker understands whole_archive_flag_spec. # This may have to be revisited, in case too many # convenience libraries get linked in and end up exceeding # the spec. if test -z "$convenience" || test -z "$whole_archive_flag_spec"; then save_libobjs=$libobjs fi save_output=$output func_basename "$output" output_la=$func_basename_result # Clear the reloadable object creation command queue and # initialize k to one. test_cmds= concat_cmds= objlist= last_robj= k=1 if test -n "$save_libobjs" && test : != "$skipped_export" && test yes = "$with_gnu_ld"; then output=$output_objdir/$output_la.lnkscript func_verbose "creating GNU ld script: $output" echo 'INPUT (' > $output for obj in $save_libobjs do func_to_tool_file "$obj" $ECHO "$func_to_tool_file_result" >> $output done echo ')' >> $output func_append delfiles " $output" func_to_tool_file "$output" output=$func_to_tool_file_result elif test -n "$save_libobjs" && test : != "$skipped_export" && test -n "$file_list_spec"; then output=$output_objdir/$output_la.lnk func_verbose "creating linker input file list: $output" : > $output set x $save_libobjs shift firstobj= if test yes = "$compiler_needs_object"; then firstobj="$1 " shift fi for obj do func_to_tool_file "$obj" $ECHO "$func_to_tool_file_result" >> $output done func_append delfiles " $output" func_to_tool_file "$output" output=$firstobj\"$file_list_spec$func_to_tool_file_result\" else if test -n "$save_libobjs"; then func_verbose "creating reloadable object files..." output=$output_objdir/$output_la-$k.$objext eval test_cmds=\"$reload_cmds\" func_len " $test_cmds" len0=$func_len_result len=$len0 # Loop over the list of objects to be linked. for obj in $save_libobjs do func_len " $obj" func_arith $len + $func_len_result len=$func_arith_result if test -z "$objlist" || test "$len" -lt "$max_cmd_len"; then func_append objlist " $obj" else # The command $test_cmds is almost too long, add a # command to the queue. if test 1 -eq "$k"; then # The first file doesn't have a previous command to add. reload_objs=$objlist eval concat_cmds=\"$reload_cmds\" else # All subsequent reloadable object files will link in # the last one created. reload_objs="$objlist $last_robj" eval concat_cmds=\"\$concat_cmds~$reload_cmds~\$RM $last_robj\" fi last_robj=$output_objdir/$output_la-$k.$objext func_arith $k + 1 k=$func_arith_result output=$output_objdir/$output_la-$k.$objext objlist=" $obj" func_len " $last_robj" func_arith $len0 + $func_len_result len=$func_arith_result fi done # Handle the remaining objects by creating one last # reloadable object file. All subsequent reloadable object # files will link in the last one created. test -z "$concat_cmds" || concat_cmds=$concat_cmds~ reload_objs="$objlist $last_robj" eval concat_cmds=\"\$concat_cmds$reload_cmds\" if test -n "$last_robj"; then eval concat_cmds=\"\$concat_cmds~\$RM $last_robj\" fi func_append delfiles " $output" else output= fi ${skipped_export-false} && { func_verbose "generating symbol list for '$libname.la'" export_symbols=$output_objdir/$libname.exp $opt_dry_run || $RM $export_symbols libobjs=$output # Append the command to create the export file. test -z "$concat_cmds" || concat_cmds=$concat_cmds~ eval concat_cmds=\"\$concat_cmds$export_symbols_cmds\" if test -n "$last_robj"; then eval concat_cmds=\"\$concat_cmds~\$RM $last_robj\" fi } test -n "$save_libobjs" && func_verbose "creating a temporary reloadable object file: $output" # Loop through the commands generated above and execute them. save_ifs=$IFS; IFS='~' for cmd in $concat_cmds; do IFS=$save_ifs $opt_quiet || { func_quote_for_expand "$cmd" eval "func_echo $func_quote_for_expand_result" } $opt_dry_run || eval "$cmd" || { lt_exit=$? # Restore the uninstalled library and exit if test relink = "$opt_mode"; then ( cd "$output_objdir" && \ $RM "${realname}T" && \ $MV "${realname}U" "$realname" ) fi exit $lt_exit } done IFS=$save_ifs if test -n "$export_symbols_regex" && ${skipped_export-false}; then func_show_eval '$EGREP -e "$export_symbols_regex" "$export_symbols" > "${export_symbols}T"' func_show_eval '$MV "${export_symbols}T" "$export_symbols"' fi fi ${skipped_export-false} && { if test -n "$export_symbols" && test -n "$include_expsyms"; then tmp_export_symbols=$export_symbols test -n "$orig_export_symbols" && tmp_export_symbols=$orig_export_symbols $opt_dry_run || eval '$ECHO "$include_expsyms" | $SP2NL >> "$tmp_export_symbols"' fi if test -n "$orig_export_symbols"; then # The given exports_symbols file has to be filtered, so filter it. func_verbose "filter symbol list for '$libname.la' to tag DATA exports" # FIXME: $output_objdir/$libname.filter potentially contains lots of # 's' commands, which not all seds can handle. GNU sed should be fine # though. Also, the filter scales superlinearly with the number of # global variables. join(1) would be nice here, but unfortunately # isn't a blessed tool. $opt_dry_run || $SED -e '/[ ,]DATA/!d;s,\(.*\)\([ \,].*\),s|^\1$|\1\2|,' < $export_symbols > $output_objdir/$libname.filter func_append delfiles " $export_symbols $output_objdir/$libname.filter" export_symbols=$output_objdir/$libname.def $opt_dry_run || $SED -f $output_objdir/$libname.filter < $orig_export_symbols > $export_symbols fi } libobjs=$output # Restore the value of output. output=$save_output if test -n "$convenience" && test -n "$whole_archive_flag_spec"; then eval libobjs=\"\$libobjs $whole_archive_flag_spec\" test "X$libobjs" = "X " && libobjs= fi # Expand the library linking commands again to reset the # value of $libobjs for piecewise linking. # Do each of the archive commands. if test yes = "$module" && test -n "$module_cmds"; then if test -n "$export_symbols" && test -n "$module_expsym_cmds"; then cmds=$module_expsym_cmds else cmds=$module_cmds fi else if test -n "$export_symbols" && test -n "$archive_expsym_cmds"; then cmds=$archive_expsym_cmds else cmds=$archive_cmds fi fi fi if test -n "$delfiles"; then # Append the command to remove temporary files to $cmds. eval cmds=\"\$cmds~\$RM $delfiles\" fi # Add any objects from preloaded convenience libraries if test -n "$dlprefiles"; then gentop=$output_objdir/${outputname}x func_append generated " $gentop" func_extract_archives $gentop $dlprefiles func_append libobjs " $func_extract_archives_result" test "X$libobjs" = "X " && libobjs= fi save_ifs=$IFS; IFS='~' for cmd in $cmds; do IFS=$sp$nl eval cmd=\"$cmd\" IFS=$save_ifs $opt_quiet || { func_quote_for_expand "$cmd" eval "func_echo $func_quote_for_expand_result" } $opt_dry_run || eval "$cmd" || { lt_exit=$? # Restore the uninstalled library and exit if test relink = "$opt_mode"; then ( cd "$output_objdir" && \ $RM "${realname}T" && \ $MV "${realname}U" "$realname" ) fi exit $lt_exit } done IFS=$save_ifs # Restore the uninstalled library and exit if test relink = "$opt_mode"; then $opt_dry_run || eval '(cd $output_objdir && $RM ${realname}T && $MV $realname ${realname}T && $MV ${realname}U $realname)' || exit $? if test -n "$convenience"; then if test -z "$whole_archive_flag_spec"; then func_show_eval '${RM}r "$gentop"' fi fi exit $EXIT_SUCCESS fi # Create links to the real library. for linkname in $linknames; do if test "$realname" != "$linkname"; then func_show_eval '(cd "$output_objdir" && $RM "$linkname" && $LN_S "$realname" "$linkname")' 'exit $?' fi done # If -module or -export-dynamic was specified, set the dlname. if test yes = "$module" || test yes = "$export_dynamic"; then # On all known operating systems, these are identical. dlname=$soname fi fi ;; obj) if test -n "$dlfiles$dlprefiles" || test no != "$dlself"; then func_warning "'-dlopen' is ignored for objects" fi case " $deplibs" in *\ -l* | *\ -L*) func_warning "'-l' and '-L' are ignored for objects" ;; esac test -n "$rpath" && \ func_warning "'-rpath' is ignored for objects" test -n "$xrpath" && \ func_warning "'-R' is ignored for objects" test -n "$vinfo" && \ func_warning "'-version-info' is ignored for objects" test -n "$release" && \ func_warning "'-release' is ignored for objects" case $output in *.lo) test -n "$objs$old_deplibs" && \ func_fatal_error "cannot build library object '$output' from non-libtool objects" libobj=$output func_lo2o "$libobj" obj=$func_lo2o_result ;; *) libobj= obj=$output ;; esac # Delete the old objects. $opt_dry_run || $RM $obj $libobj # Objects from convenience libraries. This assumes # single-version convenience libraries. Whenever we create # different ones for PIC/non-PIC, this we'll have to duplicate # the extraction. reload_conv_objs= gentop= # if reload_cmds runs $LD directly, get rid of -Wl from # whole_archive_flag_spec and hope we can get by with turning comma # into space. case $reload_cmds in *\$LD[\ \$]*) wl= ;; esac if test -n "$convenience"; then if test -n "$whole_archive_flag_spec"; then eval tmp_whole_archive_flags=\"$whole_archive_flag_spec\" test -n "$wl" || tmp_whole_archive_flags=`$ECHO "$tmp_whole_archive_flags" | $SED 's|,| |g'` reload_conv_objs=$reload_objs\ $tmp_whole_archive_flags else gentop=$output_objdir/${obj}x func_append generated " $gentop" func_extract_archives $gentop $convenience reload_conv_objs="$reload_objs $func_extract_archives_result" fi fi # If we're not building shared, we need to use non_pic_objs test yes = "$build_libtool_libs" || libobjs=$non_pic_objects # Create the old-style object. reload_objs=$objs$old_deplibs' '`$ECHO "$libobjs" | $SP2NL | $SED "/\.$libext$/d; /\.lib$/d; $lo2o" | $NL2SP`' '$reload_conv_objs output=$obj func_execute_cmds "$reload_cmds" 'exit $?' # Exit if we aren't doing a library object file. if test -z "$libobj"; then if test -n "$gentop"; then func_show_eval '${RM}r "$gentop"' fi exit $EXIT_SUCCESS fi test yes = "$build_libtool_libs" || { if test -n "$gentop"; then func_show_eval '${RM}r "$gentop"' fi # Create an invalid libtool object if no PIC, so that we don't # accidentally link it into a program. # $show "echo timestamp > $libobj" # $opt_dry_run || eval "echo timestamp > $libobj" || exit $? exit $EXIT_SUCCESS } if test -n "$pic_flag" || test default != "$pic_mode"; then # Only do commands if we really have different PIC objects. reload_objs="$libobjs $reload_conv_objs" output=$libobj func_execute_cmds "$reload_cmds" 'exit $?' fi if test -n "$gentop"; then func_show_eval '${RM}r "$gentop"' fi exit $EXIT_SUCCESS ;; prog) case $host in *cygwin*) func_stripname '' '.exe' "$output" output=$func_stripname_result.exe;; esac test -n "$vinfo" && \ func_warning "'-version-info' is ignored for programs" test -n "$release" && \ func_warning "'-release' is ignored for programs" $preload \ && test unknown,unknown,unknown = "$dlopen_support,$dlopen_self,$dlopen_self_static" \ && func_warning "'LT_INIT([dlopen])' not used. Assuming no dlopen support." case $host in *-*-rhapsody* | *-*-darwin1.[012]) # On Rhapsody replace the C library is the System framework compile_deplibs=`$ECHO " $compile_deplibs" | $SED 's/ -lc / System.ltframework /'` finalize_deplibs=`$ECHO " $finalize_deplibs" | $SED 's/ -lc / System.ltframework /'` ;; esac case $host in *-*-darwin*) # Don't allow lazy linking, it breaks C++ global constructors # But is supposedly fixed on 10.4 or later (yay!). if test CXX = "$tagname"; then case ${MACOSX_DEPLOYMENT_TARGET-10.0} in 10.[0123]) func_append compile_command " $wl-bind_at_load" func_append finalize_command " $wl-bind_at_load" ;; esac fi # Time to change all our "foo.ltframework" stuff back to "-framework foo" compile_deplibs=`$ECHO " $compile_deplibs" | $SED 's% \([^ $]*\).ltframework% -framework \1%g'` finalize_deplibs=`$ECHO " $finalize_deplibs" | $SED 's% \([^ $]*\).ltframework% -framework \1%g'` ;; esac # move library search paths that coincide with paths to not yet # installed libraries to the beginning of the library search list new_libs= for path in $notinst_path; do case " $new_libs " in *" -L$path/$objdir "*) ;; *) case " $compile_deplibs " in *" -L$path/$objdir "*) func_append new_libs " -L$path/$objdir" ;; esac ;; esac done for deplib in $compile_deplibs; do case $deplib in -L*) case " $new_libs " in *" $deplib "*) ;; *) func_append new_libs " $deplib" ;; esac ;; *) func_append new_libs " $deplib" ;; esac done compile_deplibs=$new_libs func_append compile_command " $compile_deplibs" func_append finalize_command " $finalize_deplibs" if test -n "$rpath$xrpath"; then # If the user specified any rpath flags, then add them. for libdir in $rpath $xrpath; do # This is the magic to use -rpath. case "$finalize_rpath " in *" $libdir "*) ;; *) func_append finalize_rpath " $libdir" ;; esac done fi # Now hardcode the library paths rpath= hardcode_libdirs= for libdir in $compile_rpath $finalize_rpath; do if test -n "$hardcode_libdir_flag_spec"; then if test -n "$hardcode_libdir_separator"; then if test -z "$hardcode_libdirs"; then hardcode_libdirs=$libdir else # Just accumulate the unique libdirs. case $hardcode_libdir_separator$hardcode_libdirs$hardcode_libdir_separator in *"$hardcode_libdir_separator$libdir$hardcode_libdir_separator"*) ;; *) func_append hardcode_libdirs "$hardcode_libdir_separator$libdir" ;; esac fi else eval flag=\"$hardcode_libdir_flag_spec\" func_append rpath " $flag" fi elif test -n "$runpath_var"; then case "$perm_rpath " in *" $libdir "*) ;; *) func_append perm_rpath " $libdir" ;; esac fi case $host in *-*-cygwin* | *-*-mingw* | *-*-pw32* | *-*-os2* | *-cegcc*) testbindir=`$ECHO "$libdir" | $SED -e 's*/lib$*/bin*'` case :$dllsearchpath: in *":$libdir:"*) ;; ::) dllsearchpath=$libdir;; *) func_append dllsearchpath ":$libdir";; esac case :$dllsearchpath: in *":$testbindir:"*) ;; ::) dllsearchpath=$testbindir;; *) func_append dllsearchpath ":$testbindir";; esac ;; esac done # Substitute the hardcoded libdirs into the rpath. if test -n "$hardcode_libdir_separator" && test -n "$hardcode_libdirs"; then libdir=$hardcode_libdirs eval rpath=\" $hardcode_libdir_flag_spec\" fi compile_rpath=$rpath rpath= hardcode_libdirs= for libdir in $finalize_rpath; do if test -n "$hardcode_libdir_flag_spec"; then if test -n "$hardcode_libdir_separator"; then if test -z "$hardcode_libdirs"; then hardcode_libdirs=$libdir else # Just accumulate the unique libdirs. case $hardcode_libdir_separator$hardcode_libdirs$hardcode_libdir_separator in *"$hardcode_libdir_separator$libdir$hardcode_libdir_separator"*) ;; *) func_append hardcode_libdirs "$hardcode_libdir_separator$libdir" ;; esac fi else eval flag=\"$hardcode_libdir_flag_spec\" func_append rpath " $flag" fi elif test -n "$runpath_var"; then case "$finalize_perm_rpath " in *" $libdir "*) ;; *) func_append finalize_perm_rpath " $libdir" ;; esac fi done # Substitute the hardcoded libdirs into the rpath. if test -n "$hardcode_libdir_separator" && test -n "$hardcode_libdirs"; then libdir=$hardcode_libdirs eval rpath=\" $hardcode_libdir_flag_spec\" fi finalize_rpath=$rpath if test -n "$libobjs" && test yes = "$build_old_libs"; then # Transform all the library objects into standard objects. compile_command=`$ECHO "$compile_command" | $SP2NL | $SED "$lo2o" | $NL2SP` finalize_command=`$ECHO "$finalize_command" | $SP2NL | $SED "$lo2o" | $NL2SP` fi func_generate_dlsyms "$outputname" "@PROGRAM@" false # template prelinking step if test -n "$prelink_cmds"; then func_execute_cmds "$prelink_cmds" 'exit $?' fi wrappers_required=: case $host in *cegcc* | *mingw32ce*) # Disable wrappers for cegcc and mingw32ce hosts, we are cross compiling anyway. wrappers_required=false ;; *cygwin* | *mingw* ) test yes = "$build_libtool_libs" || wrappers_required=false ;; *) if test no = "$need_relink" || test yes != "$build_libtool_libs"; then wrappers_required=false fi ;; esac $wrappers_required || { # Replace the output file specification. compile_command=`$ECHO "$compile_command" | $SED 's%@OUTPUT@%'"$output"'%g'` link_command=$compile_command$compile_rpath # We have no uninstalled library dependencies, so finalize right now. exit_status=0 func_show_eval "$link_command" 'exit_status=$?' if test -n "$postlink_cmds"; then func_to_tool_file "$output" postlink_cmds=`func_echo_all "$postlink_cmds" | $SED -e 's%@OUTPUT@%'"$output"'%g' -e 's%@TOOL_OUTPUT@%'"$func_to_tool_file_result"'%g'` func_execute_cmds "$postlink_cmds" 'exit $?' fi # Delete the generated files. if test -f "$output_objdir/${outputname}S.$objext"; then func_show_eval '$RM "$output_objdir/${outputname}S.$objext"' fi exit $exit_status } if test -n "$compile_shlibpath$finalize_shlibpath"; then compile_command="$shlibpath_var=\"$compile_shlibpath$finalize_shlibpath\$$shlibpath_var\" $compile_command" fi if test -n "$finalize_shlibpath"; then finalize_command="$shlibpath_var=\"$finalize_shlibpath\$$shlibpath_var\" $finalize_command" fi compile_var= finalize_var= if test -n "$runpath_var"; then if test -n "$perm_rpath"; then # We should set the runpath_var. rpath= for dir in $perm_rpath; do func_append rpath "$dir:" done compile_var="$runpath_var=\"$rpath\$$runpath_var\" " fi if test -n "$finalize_perm_rpath"; then # We should set the runpath_var. rpath= for dir in $finalize_perm_rpath; do func_append rpath "$dir:" done finalize_var="$runpath_var=\"$rpath\$$runpath_var\" " fi fi if test yes = "$no_install"; then # We don't need to create a wrapper script. link_command=$compile_var$compile_command$compile_rpath # Replace the output file specification. link_command=`$ECHO "$link_command" | $SED 's%@OUTPUT@%'"$output"'%g'` # Delete the old output file. $opt_dry_run || $RM $output # Link the executable and exit func_show_eval "$link_command" 'exit $?' if test -n "$postlink_cmds"; then func_to_tool_file "$output" postlink_cmds=`func_echo_all "$postlink_cmds" | $SED -e 's%@OUTPUT@%'"$output"'%g' -e 's%@TOOL_OUTPUT@%'"$func_to_tool_file_result"'%g'` func_execute_cmds "$postlink_cmds" 'exit $?' fi exit $EXIT_SUCCESS fi case $hardcode_action,$fast_install in relink,*) # Fast installation is not supported link_command=$compile_var$compile_command$compile_rpath relink_command=$finalize_var$finalize_command$finalize_rpath func_warning "this platform does not like uninstalled shared libraries" func_warning "'$output' will be relinked during installation" ;; *,yes) link_command=$finalize_var$compile_command$finalize_rpath relink_command=`$ECHO "$compile_var$compile_command$compile_rpath" | $SED 's%@OUTPUT@%\$progdir/\$file%g'` ;; *,no) link_command=$compile_var$compile_command$compile_rpath relink_command=$finalize_var$finalize_command$finalize_rpath ;; *,needless) link_command=$finalize_var$compile_command$finalize_rpath relink_command= ;; esac # Replace the output file specification. link_command=`$ECHO "$link_command" | $SED 's%@OUTPUT@%'"$output_objdir/$outputname"'%g'` # Delete the old output files. $opt_dry_run || $RM $output $output_objdir/$outputname $output_objdir/lt-$outputname func_show_eval "$link_command" 'exit $?' if test -n "$postlink_cmds"; then func_to_tool_file "$output_objdir/$outputname" postlink_cmds=`func_echo_all "$postlink_cmds" | $SED -e 's%@OUTPUT@%'"$output_objdir/$outputname"'%g' -e 's%@TOOL_OUTPUT@%'"$func_to_tool_file_result"'%g'` func_execute_cmds "$postlink_cmds" 'exit $?' fi # Now create the wrapper script. func_verbose "creating $output" # Quote the relink command for shipping. if test -n "$relink_command"; then # Preserve any variables that may affect compiler behavior for var in $variables_saved_for_relink; do if eval test -z \"\${$var+set}\"; then relink_command="{ test -z \"\${$var+set}\" || $lt_unset $var || { $var=; export $var; }; }; $relink_command" elif eval var_value=\$$var; test -z "$var_value"; then relink_command="$var=; export $var; $relink_command" else func_quote_for_eval "$var_value" relink_command="$var=$func_quote_for_eval_result; export $var; $relink_command" fi done relink_command="(cd `pwd`; $relink_command)" relink_command=`$ECHO "$relink_command" | $SED "$sed_quote_subst"` fi # Only actually do things if not in dry run mode. $opt_dry_run || { # win32 will think the script is a binary if it has # a .exe suffix, so we strip it off here. case $output in *.exe) func_stripname '' '.exe' "$output" output=$func_stripname_result ;; esac # test for cygwin because mv fails w/o .exe extensions case $host in *cygwin*) exeext=.exe func_stripname '' '.exe' "$outputname" outputname=$func_stripname_result ;; *) exeext= ;; esac case $host in *cygwin* | *mingw* ) func_dirname_and_basename "$output" "" "." output_name=$func_basename_result output_path=$func_dirname_result cwrappersource=$output_path/$objdir/lt-$output_name.c cwrapper=$output_path/$output_name.exe $RM $cwrappersource $cwrapper trap "$RM $cwrappersource $cwrapper; exit $EXIT_FAILURE" 1 2 15 func_emit_cwrapperexe_src > $cwrappersource # The wrapper executable is built using the $host compiler, # because it contains $host paths and files. If cross- # compiling, it, like the target executable, must be # executed on the $host or under an emulation environment. $opt_dry_run || { $LTCC $LTCFLAGS -o $cwrapper $cwrappersource $STRIP $cwrapper } # Now, create the wrapper script for func_source use: func_ltwrapper_scriptname $cwrapper $RM $func_ltwrapper_scriptname_result trap "$RM $func_ltwrapper_scriptname_result; exit $EXIT_FAILURE" 1 2 15 $opt_dry_run || { # note: this script will not be executed, so do not chmod. if test "x$build" = "x$host"; then $cwrapper --lt-dump-script > $func_ltwrapper_scriptname_result else func_emit_wrapper no > $func_ltwrapper_scriptname_result fi } ;; * ) $RM $output trap "$RM $output; exit $EXIT_FAILURE" 1 2 15 func_emit_wrapper no > $output chmod +x $output ;; esac } exit $EXIT_SUCCESS ;; esac # See if we need to build an old-fashioned archive. for oldlib in $oldlibs; do case $build_libtool_libs in convenience) oldobjs="$libobjs_save $symfileobj" addlibs=$convenience build_libtool_libs=no ;; module) oldobjs=$libobjs_save addlibs=$old_convenience build_libtool_libs=no ;; *) oldobjs="$old_deplibs $non_pic_objects" $preload && test -f "$symfileobj" \ && func_append oldobjs " $symfileobj" addlibs=$old_convenience ;; esac if test -n "$addlibs"; then gentop=$output_objdir/${outputname}x func_append generated " $gentop" func_extract_archives $gentop $addlibs func_append oldobjs " $func_extract_archives_result" fi # Do each command in the archive commands. if test -n "$old_archive_from_new_cmds" && test yes = "$build_libtool_libs"; then cmds=$old_archive_from_new_cmds else # Add any objects from preloaded convenience libraries if test -n "$dlprefiles"; then gentop=$output_objdir/${outputname}x func_append generated " $gentop" func_extract_archives $gentop $dlprefiles func_append oldobjs " $func_extract_archives_result" fi # POSIX demands no paths to be encoded in archives. We have # to avoid creating archives with duplicate basenames if we # might have to extract them afterwards, e.g., when creating a # static archive out of a convenience library, or when linking # the entirety of a libtool archive into another (currently # not supported by libtool). if (for obj in $oldobjs do func_basename "$obj" $ECHO "$func_basename_result" done | sort | sort -uc >/dev/null 2>&1); then : else echo "copying selected object files to avoid basename conflicts..." gentop=$output_objdir/${outputname}x func_append generated " $gentop" func_mkdir_p "$gentop" save_oldobjs=$oldobjs oldobjs= counter=1 for obj in $save_oldobjs do func_basename "$obj" objbase=$func_basename_result case " $oldobjs " in " ") oldobjs=$obj ;; *[\ /]"$objbase "*) while :; do # Make sure we don't pick an alternate name that also # overlaps. newobj=lt$counter-$objbase func_arith $counter + 1 counter=$func_arith_result case " $oldobjs " in *[\ /]"$newobj "*) ;; *) if test ! -f "$gentop/$newobj"; then break; fi ;; esac done func_show_eval "ln $obj $gentop/$newobj || cp $obj $gentop/$newobj" func_append oldobjs " $gentop/$newobj" ;; *) func_append oldobjs " $obj" ;; esac done fi func_to_tool_file "$oldlib" func_convert_file_msys_to_w32 tool_oldlib=$func_to_tool_file_result eval cmds=\"$old_archive_cmds\" func_len " $cmds" len=$func_len_result if test "$len" -lt "$max_cmd_len" || test "$max_cmd_len" -le -1; then cmds=$old_archive_cmds elif test -n "$archiver_list_spec"; then func_verbose "using command file archive linking..." for obj in $oldobjs do func_to_tool_file "$obj" $ECHO "$func_to_tool_file_result" done > $output_objdir/$libname.libcmd func_to_tool_file "$output_objdir/$libname.libcmd" oldobjs=" $archiver_list_spec$func_to_tool_file_result" cmds=$old_archive_cmds else # the command line is too long to link in one step, link in parts func_verbose "using piecewise archive linking..." save_RANLIB=$RANLIB RANLIB=: objlist= concat_cmds= save_oldobjs=$oldobjs oldobjs= # Is there a better way of finding the last object in the list? 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See the GNU # General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program; if not, see <http://www.gnu.org/licenses/>. # # As a special exception to the GNU General Public License, if you # distribute this file as part of a program that contains a # configuration script generated by Autoconf, you may include it under # the same distribution terms that you use for the rest of that # program. This Exception is an additional permission under section 7 # of the GNU General Public License, version 3 ("GPLv3"). # Please send patches to <config-patches@gnu.org>. # # Configuration subroutine to validate and canonicalize a configuration type. # Supply the specified configuration type as an argument. # If it is invalid, we print an error message on stderr and exit with code 1. # Otherwise, we print the canonical config type on stdout and succeed. # You can get the latest version of this script from: # http://git.savannah.gnu.org/gitweb/?p=config.git;a=blob_plain;f=config.sub # This file is supposed to be the same for all GNU packages # and recognize all the CPU types, system types and aliases # that are meaningful with *any* GNU software. # Each package is responsible for reporting which valid configurations # it does not support. The user should be able to distinguish # a failure to support a valid configuration from a meaningless # configuration. # The goal of this file is to map all the various variations of a given # machine specification into a single specification in the form: # CPU_TYPE-MANUFACTURER-OPERATING_SYSTEM # or in some cases, the newer four-part form: # CPU_TYPE-MANUFACTURER-KERNEL-OPERATING_SYSTEM # It is wrong to echo any other type of specification. me=`echo "$0" | sed -e 's,.*/,,'` usage="\ Usage: $0 [OPTION] CPU-MFR-OPSYS or ALIAS Canonicalize a configuration name. Operation modes: -h, --help print this help, then exit -t, --time-stamp print date of last modification, then exit -v, --version print version number, then exit Report bugs and patches to <config-patches@gnu.org>." version="\ GNU config.sub ($timestamp) Copyright 1992-2016 Free Software Foundation, Inc. This is free software; see the source for copying conditions. There is NO warranty; not even for MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE." help=" Try \`$me --help' for more information." # Parse command line while test $# -gt 0 ; do case $1 in --time-stamp | --time* | -t ) echo "$timestamp" ; exit ;; --version | -v ) echo "$version" ; exit ;; --help | --h* | -h ) echo "$usage"; exit ;; -- ) # Stop option processing shift; break ;; - ) # Use stdin as input. break ;; -* ) echo "$me: invalid option $1$help" exit 1 ;; *local*) # First pass through any local machine types. echo $1 exit ;; * ) break ;; esac done case $# in 0) echo "$me: missing argument$help" >&2 exit 1;; 1) ;; *) echo "$me: too many arguments$help" >&2 exit 1;; esac # Separate what the user gave into CPU-COMPANY and OS or KERNEL-OS (if any). # Here we must recognize all the valid KERNEL-OS combinations. maybe_os=`echo $1 | sed 's/^\(.*\)-\([^-]*-[^-]*\)$/\2/'` case $maybe_os in nto-qnx* | linux-gnu* | linux-android* | linux-dietlibc | linux-newlib* | \ linux-musl* | linux-uclibc* | uclinux-uclibc* | uclinux-gnu* | kfreebsd*-gnu* | \ knetbsd*-gnu* | netbsd*-gnu* | netbsd*-eabi* | \ kopensolaris*-gnu* | cloudabi*-eabi* | \ storm-chaos* | os2-emx* | rtmk-nova*) os=-$maybe_os basic_machine=`echo $1 | sed 's/^\(.*\)-\([^-]*-[^-]*\)$/\1/'` ;; android-linux) os=-linux-android basic_machine=`echo $1 | sed 's/^\(.*\)-\([^-]*-[^-]*\)$/\1/'`-unknown ;; *) basic_machine=`echo $1 | sed 's/-[^-]*$//'` if [ $basic_machine != $1 ] then os=`echo $1 | sed 's/.*-/-/'` else os=; fi ;; esac ### Let's recognize common machines as not being operating systems so ### that things like config.sub decstation-3100 work. We also ### recognize some manufacturers as not being operating systems, so we ### can provide default operating systems below. case $os in -sun*os*) # Prevent following clause from handling this invalid input. ;; -dec* | -mips* | -sequent* | -encore* | -pc532* | -sgi* | -sony* | \ -att* | -7300* | -3300* | -delta* | -motorola* | -sun[234]* | \ -unicom* | -ibm* | -next | -hp | -isi* | -apollo | -altos* | \ -convergent* | -ncr* | -news | -32* | -3600* | -3100* | -hitachi* |\ -c[123]* | -convex* | -sun | -crds | -omron* | -dg | -ultra | -tti* | \ -harris | -dolphin | -highlevel | -gould | -cbm | -ns | -masscomp | \ -apple | -axis | -knuth | -cray | -microblaze*) os= basic_machine=$1 ;; -bluegene*) os=-cnk ;; -sim | -cisco | -oki | -wec | -winbond) os= basic_machine=$1 ;; -scout) ;; -wrs) os=-vxworks basic_machine=$1 ;; -chorusos*) os=-chorusos basic_machine=$1 ;; -chorusrdb) os=-chorusrdb basic_machine=$1 ;; -hiux*) os=-hiuxwe2 ;; -sco6) os=-sco5v6 basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco5) os=-sco3.2v5 basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco4) os=-sco3.2v4 basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco3.2.[4-9]*) os=`echo $os | sed -e 's/sco3.2./sco3.2v/'` basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco3.2v[4-9]*) # Don't forget version if it is 3.2v4 or newer. basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco5v6*) # Don't forget version if it is 3.2v4 or newer. basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco*) os=-sco3.2v2 basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -udk*) basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -isc) os=-isc2.2 basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -clix*) basic_machine=clipper-intergraph ;; -isc*) basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -lynx*178) os=-lynxos178 ;; -lynx*5) os=-lynxos5 ;; -lynx*) os=-lynxos ;; -ptx*) basic_machine=`echo $1 | sed -e 's/86-.*/86-sequent/'` ;; -windowsnt*) os=`echo $os | sed -e 's/windowsnt/winnt/'` ;; -psos*) os=-psos ;; -mint | -mint[0-9]*) basic_machine=m68k-atari os=-mint ;; esac # Decode aliases for certain CPU-COMPANY combinations. case $basic_machine in # Recognize the basic CPU types without company name. # Some are omitted here because they have special meanings below. 1750a | 580 \ | a29k \ | aarch64 | aarch64_be \ | alpha | alphaev[4-8] | alphaev56 | alphaev6[78] | alphapca5[67] \ | alpha64 | alpha64ev[4-8] | alpha64ev56 | alpha64ev6[78] | alpha64pca5[67] \ | am33_2.0 \ | arc | arceb \ | arm | arm[bl]e | arme[lb] | armv[2-8] | armv[3-8][lb] | armv7[arm] \ | avr | avr32 \ | ba \ | be32 | be64 \ | bfin \ | c4x | c8051 | clipper \ | d10v | d30v | dlx | dsp16xx \ | e2k | epiphany \ | fido | fr30 | frv | ft32 \ | h8300 | h8500 | hppa | hppa1.[01] | hppa2.0 | hppa2.0[nw] | hppa64 \ | hexagon \ | i370 | i860 | i960 | ia64 \ | ip2k | iq2000 \ | k1om \ | le32 | le64 \ | lm32 \ | m32c | m32r | m32rle | m68000 | m68k | m88k \ | maxq | mb | microblaze | microblazeel | mcore | mep | metag \ | mips | mipsbe | mipseb | mipsel | mipsle \ | mips16 \ | mips64 | mips64el \ | mips64octeon | mips64octeonel \ | mips64orion | mips64orionel \ | mips64r5900 | mips64r5900el \ | mips64vr | mips64vrel \ | mips64vr4100 | mips64vr4100el \ | mips64vr4300 | mips64vr4300el \ | mips64vr5000 | mips64vr5000el \ | mips64vr5900 | mips64vr5900el \ | mipsisa32 | mipsisa32el \ | mipsisa32r2 | mipsisa32r2el \ | mipsisa32r6 | mipsisa32r6el \ | mipsisa64 | mipsisa64el \ | mipsisa64r2 | mipsisa64r2el \ | mipsisa64r6 | mipsisa64r6el \ | mipsisa64sb1 | mipsisa64sb1el \ | mipsisa64sr71k | mipsisa64sr71kel \ | mipsr5900 | mipsr5900el \ | mipstx39 | mipstx39el \ | mn10200 | mn10300 \ | moxie \ | mt \ | msp430 \ | nds32 | nds32le | nds32be \ | nios | nios2 | nios2eb | nios2el \ | ns16k | ns32k \ | open8 | or1k | or1knd | or32 \ | pdp10 | pdp11 | pj | pjl \ | powerpc | powerpc64 | powerpc64le | powerpcle \ | pyramid \ | riscv32 | riscv64 \ | rl78 | rx \ | score \ | sh | sh[1234] | sh[24]a | sh[24]aeb | sh[23]e | sh[234]eb | sheb | shbe | shle | sh[1234]le | sh3ele \ | sh64 | sh64le \ | sparc | sparc64 | sparc64b | sparc64v | sparc86x | sparclet | sparclite \ | sparcv8 | sparcv9 | sparcv9b | sparcv9v \ | spu \ | tahoe | tic4x | tic54x | tic55x | tic6x | tic80 | tron \ | ubicom32 \ | v850 | v850e | v850e1 | v850e2 | v850es | v850e2v3 \ | visium \ | we32k \ | x86 | xc16x | xstormy16 | xtensa \ | z8k | z80) basic_machine=$basic_machine-unknown ;; c54x) basic_machine=tic54x-unknown ;; c55x) basic_machine=tic55x-unknown ;; c6x) basic_machine=tic6x-unknown ;; leon|leon[3-9]) basic_machine=sparc-$basic_machine ;; m6811 | m68hc11 | m6812 | m68hc12 | m68hcs12x | nvptx | picochip) basic_machine=$basic_machine-unknown os=-none ;; m88110 | m680[12346]0 | m683?2 | m68360 | m5200 | v70 | w65 | z8k) ;; ms1) basic_machine=mt-unknown ;; strongarm | thumb | xscale) basic_machine=arm-unknown ;; xgate) basic_machine=$basic_machine-unknown os=-none ;; xscaleeb) basic_machine=armeb-unknown ;; xscaleel) basic_machine=armel-unknown ;; # We use `pc' rather than `unknown' # because (1) that's what they normally are, and # (2) the word "unknown" tends to confuse beginning users. i*86 | x86_64) basic_machine=$basic_machine-pc ;; # Object if more than one company name word. *-*-*) echo Invalid configuration \`$1\': machine \`$basic_machine\' not recognized 1>&2 exit 1 ;; # Recognize the basic CPU types with company name. 580-* \ | a29k-* \ | aarch64-* | aarch64_be-* \ | alpha-* | alphaev[4-8]-* | alphaev56-* | alphaev6[78]-* \ | alpha64-* | alpha64ev[4-8]-* | alpha64ev56-* | alpha64ev6[78]-* \ | alphapca5[67]-* | alpha64pca5[67]-* | arc-* | arceb-* \ | arm-* | armbe-* | armle-* | armeb-* | armv*-* \ | avr-* | avr32-* \ | ba-* \ | be32-* | be64-* \ | bfin-* | bs2000-* \ | c[123]* | c30-* | [cjt]90-* | c4x-* \ | c8051-* | clipper-* | craynv-* | cydra-* \ | d10v-* | d30v-* | dlx-* \ | e2k-* | elxsi-* \ | f30[01]-* | f700-* | fido-* | fr30-* | frv-* | fx80-* \ | h8300-* | h8500-* \ | hppa-* | hppa1.[01]-* | hppa2.0-* | hppa2.0[nw]-* | hppa64-* \ | hexagon-* \ | i*86-* | i860-* | i960-* | ia64-* \ | ip2k-* | iq2000-* \ | k1om-* \ | le32-* | le64-* \ | lm32-* \ | m32c-* | m32r-* | m32rle-* \ | m68000-* | m680[012346]0-* | m68360-* | m683?2-* | m68k-* \ | m88110-* | m88k-* | maxq-* | mcore-* | metag-* \ | microblaze-* | microblazeel-* \ | mips-* | mipsbe-* | mipseb-* | mipsel-* | mipsle-* \ | mips16-* \ | mips64-* | mips64el-* \ | mips64octeon-* | mips64octeonel-* \ | mips64orion-* | mips64orionel-* \ | mips64r5900-* | mips64r5900el-* \ | mips64vr-* | mips64vrel-* \ | mips64vr4100-* | mips64vr4100el-* \ | mips64vr4300-* | mips64vr4300el-* \ | mips64vr5000-* | mips64vr5000el-* \ | mips64vr5900-* | mips64vr5900el-* \ | mipsisa32-* | mipsisa32el-* \ | mipsisa32r2-* | mipsisa32r2el-* \ | mipsisa32r6-* | mipsisa32r6el-* \ | mipsisa64-* | mipsisa64el-* \ | mipsisa64r2-* | mipsisa64r2el-* \ | mipsisa64r6-* | mipsisa64r6el-* \ | mipsisa64sb1-* | mipsisa64sb1el-* \ | mipsisa64sr71k-* | mipsisa64sr71kel-* \ | mipsr5900-* | mipsr5900el-* \ | mipstx39-* | mipstx39el-* \ | mmix-* \ | mt-* \ | msp430-* \ | nds32-* | nds32le-* | nds32be-* \ | nios-* | nios2-* | nios2eb-* | nios2el-* \ | none-* | np1-* | ns16k-* | ns32k-* \ | open8-* \ | or1k*-* \ | orion-* \ | pdp10-* | pdp11-* | pj-* | pjl-* | pn-* | power-* \ | powerpc-* | powerpc64-* | powerpc64le-* | powerpcle-* \ | pyramid-* \ | riscv32-* | riscv64-* \ | rl78-* | romp-* | rs6000-* | rx-* \ | sh-* | sh[1234]-* | sh[24]a-* | sh[24]aeb-* | sh[23]e-* | sh[34]eb-* | sheb-* | shbe-* \ | shle-* | sh[1234]le-* | sh3ele-* | sh64-* | sh64le-* \ | sparc-* | sparc64-* | sparc64b-* | sparc64v-* | sparc86x-* | sparclet-* \ | sparclite-* \ | sparcv8-* | sparcv9-* | sparcv9b-* | sparcv9v-* | sv1-* | sx*-* \ | tahoe-* \ | tic30-* | tic4x-* | tic54x-* | tic55x-* | tic6x-* | tic80-* \ | tile*-* \ | tron-* \ | ubicom32-* \ | v850-* | v850e-* | v850e1-* | v850es-* | v850e2-* | v850e2v3-* \ | vax-* \ | visium-* \ | we32k-* \ | x86-* | x86_64-* | xc16x-* | xps100-* \ | xstormy16-* | xtensa*-* \ | ymp-* \ | z8k-* | z80-*) ;; # Recognize the basic CPU types without company name, with glob match. xtensa*) basic_machine=$basic_machine-unknown ;; # Recognize the various machine names and aliases which stand # for a CPU type and a company and sometimes even an OS. 386bsd) basic_machine=i386-unknown os=-bsd ;; 3b1 | 7300 | 7300-att | att-7300 | pc7300 | safari | unixpc) basic_machine=m68000-att ;; 3b*) basic_machine=we32k-att ;; a29khif) basic_machine=a29k-amd os=-udi ;; abacus) basic_machine=abacus-unknown ;; adobe68k) basic_machine=m68010-adobe os=-scout ;; alliant | fx80) basic_machine=fx80-alliant ;; altos | altos3068) basic_machine=m68k-altos ;; am29k) basic_machine=a29k-none os=-bsd ;; amd64) basic_machine=x86_64-pc ;; amd64-*) basic_machine=x86_64-`echo $basic_machine | sed 's/^[^-]*-//'` ;; amdahl) basic_machine=580-amdahl os=-sysv ;; amiga | amiga-*) basic_machine=m68k-unknown ;; amigaos | amigados) basic_machine=m68k-unknown os=-amigaos ;; amigaunix | amix) basic_machine=m68k-unknown os=-sysv4 ;; apollo68) basic_machine=m68k-apollo os=-sysv ;; apollo68bsd) basic_machine=m68k-apollo os=-bsd ;; aros) basic_machine=i386-pc os=-aros ;; asmjs) basic_machine=asmjs-unknown ;; aux) basic_machine=m68k-apple os=-aux ;; balance) basic_machine=ns32k-sequent os=-dynix ;; blackfin) basic_machine=bfin-unknown os=-linux ;; blackfin-*) basic_machine=bfin-`echo $basic_machine | sed 's/^[^-]*-//'` os=-linux ;; bluegene*) basic_machine=powerpc-ibm os=-cnk ;; c54x-*) basic_machine=tic54x-`echo $basic_machine | sed 's/^[^-]*-//'` ;; c55x-*) basic_machine=tic55x-`echo $basic_machine | sed 's/^[^-]*-//'` ;; c6x-*) basic_machine=tic6x-`echo $basic_machine | sed 's/^[^-]*-//'` ;; c90) basic_machine=c90-cray os=-unicos ;; cegcc) basic_machine=arm-unknown os=-cegcc ;; convex-c1) basic_machine=c1-convex os=-bsd ;; convex-c2) basic_machine=c2-convex os=-bsd ;; convex-c32) basic_machine=c32-convex os=-bsd ;; convex-c34) basic_machine=c34-convex os=-bsd ;; convex-c38) basic_machine=c38-convex os=-bsd ;; cray | j90) basic_machine=j90-cray os=-unicos ;; craynv) basic_machine=craynv-cray os=-unicosmp ;; 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We still # use `HOST_CC' if defined, but it is deprecated. # Portable tmp directory creation inspired by the Autoconf team. set_cc_for_build=' trap "exitcode=\$?; (rm -f \$tmpfiles 2>/dev/null; rmdir \$tmp 2>/dev/null) && exit \$exitcode" 0 ; trap "rm -f \$tmpfiles 2>/dev/null; rmdir \$tmp 2>/dev/null; exit 1" 1 2 13 15 ; : ${TMPDIR=/tmp} ; { tmp=`(umask 077 && mktemp -d "$TMPDIR/cgXXXXXX") 2>/dev/null` && test -n "$tmp" && test -d "$tmp" ; } || { test -n "$RANDOM" && tmp=$TMPDIR/cg$$-$RANDOM && (umask 077 && mkdir $tmp) ; } || { tmp=$TMPDIR/cg-$$ && (umask 077 && mkdir $tmp) && echo "Warning: creating insecure temp directory" >&2 ; } || { echo "$me: cannot create a temporary directory in $TMPDIR" >&2 ; exit 1 ; } ; dummy=$tmp/dummy ; tmpfiles="$dummy.c $dummy.o $dummy.rel $dummy" ; case $CC_FOR_BUILD,$HOST_CC,$CC in ,,) echo "int x;" > $dummy.c ; for c in cc gcc c89 c99 ; do if ($c -c -o $dummy.o $dummy.c) >/dev/null 2>&1 ; then CC_FOR_BUILD="$c"; break ; fi ; done ; if test x"$CC_FOR_BUILD" = x ; then CC_FOR_BUILD=no_compiler_found ; fi ;; ,,*) CC_FOR_BUILD=$CC ;; ,*,*) CC_FOR_BUILD=$HOST_CC ;; esac ; set_cc_for_build= ;' # This is needed to find uname on a Pyramid OSx when run in the BSD universe. # (ghazi@noc.rutgers.edu 1994-08-24) if (test -f /.attbin/uname) >/dev/null 2>&1 ; then PATH=$PATH:/.attbin ; export PATH fi UNAME_MACHINE=`(uname -m) 2>/dev/null` || UNAME_MACHINE=unknown UNAME_RELEASE=`(uname -r) 2>/dev/null` || UNAME_RELEASE=unknown UNAME_SYSTEM=`(uname -s) 2>/dev/null` || UNAME_SYSTEM=unknown UNAME_VERSION=`(uname -v) 2>/dev/null` || UNAME_VERSION=unknown case "${UNAME_SYSTEM}" in Linux|GNU|GNU/*) # If the system lacks a compiler, then just pick glibc. # We could probably try harder. LIBC=gnu eval $set_cc_for_build cat <<-EOF > $dummy.c #include <features.h> #if defined(__UCLIBC__) LIBC=uclibc #elif defined(__dietlibc__) LIBC=dietlibc #else LIBC=gnu #endif EOF eval `$CC_FOR_BUILD -E $dummy.c 2>/dev/null | grep '^LIBC' | sed 's, ,,g'` ;; esac # Note: order is significant - the case branches are not exclusive. case "${UNAME_MACHINE}:${UNAME_SYSTEM}:${UNAME_RELEASE}:${UNAME_VERSION}" in *:NetBSD:*:*) # NetBSD (nbsd) targets should (where applicable) match one or # more of the tuples: *-*-netbsdelf*, *-*-netbsdaout*, # *-*-netbsdecoff* and *-*-netbsd*. For targets that recently # switched to ELF, *-*-netbsd* would select the old # object file format. This provides both forward # compatibility and a consistent mechanism for selecting the # object file format. # # Note: NetBSD doesn't particularly care about the vendor # portion of the name. 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Ake) contributed MIS and NILE. if test "`(/bin/universe) 2>/dev/null`" = att ; then echo pyramid-pyramid-sysv3 else echo pyramid-pyramid-bsd fi exit ;; NILE*:*:*:dcosx) echo pyramid-pyramid-svr4 exit ;; DRS?6000:unix:4.0:6*) echo sparc-icl-nx6 exit ;; DRS?6000:UNIX_SV:4.2*:7* | DRS?6000:isis:4.2*:7*) case `/usr/bin/uname -p` in sparc) echo sparc-icl-nx7; exit ;; esac ;; s390x:SunOS:*:*) echo ${UNAME_MACHINE}-ibm-solaris2`echo ${UNAME_RELEASE}|sed -e 's/[^.]*//'` exit ;; sun4H:SunOS:5.*:*) echo sparc-hal-solaris2`echo ${UNAME_RELEASE}|sed -e 's/[^.]*//'` exit ;; sun4*:SunOS:5.*:* | tadpole*:SunOS:5.*:*) echo sparc-sun-solaris2`echo ${UNAME_RELEASE}|sed -e 's/[^.]*//'` exit ;; i86pc:AuroraUX:5.*:* | i86xen:AuroraUX:5.*:*) echo i386-pc-auroraux${UNAME_RELEASE} exit ;; i86pc:SunOS:5.*:* | i86xen:SunOS:5.*:*) eval $set_cc_for_build SUN_ARCH=i386 # If there is a compiler, see if it is configured for 64-bit objects. # Note that the Sun cc does not turn __LP64__ into 1 like gcc does. # This test works for both compilers. if [ "$CC_FOR_BUILD" != no_compiler_found ]; then if (echo '#ifdef __amd64'; echo IS_64BIT_ARCH; echo '#endif') | \ (CCOPTS="" $CC_FOR_BUILD -E - 2>/dev/null) | \ grep IS_64BIT_ARCH >/dev/null then SUN_ARCH=x86_64 fi fi echo ${SUN_ARCH}-pc-solaris2`echo ${UNAME_RELEASE}|sed -e 's/[^.]*//'` exit ;; sun4*:SunOS:6*:*) # According to config.sub, this is the proper way to canonicalize # SunOS6. 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The system name ranges from "MiNT" over "FreeMiNT" # to the lowercase version "mint" (or "freemint"). Finally # the system name "TOS" denotes a system which is actually not # MiNT. But MiNT is downward compatible to TOS, so this should # be no problem. atarist[e]:*MiNT:*:* | atarist[e]:*mint:*:* | atarist[e]:*TOS:*:*) echo m68k-atari-mint${UNAME_RELEASE} exit ;; atari*:*MiNT:*:* | atari*:*mint:*:* | atarist[e]:*TOS:*:*) echo m68k-atari-mint${UNAME_RELEASE} exit ;; *falcon*:*MiNT:*:* | *falcon*:*mint:*:* | *falcon*:*TOS:*:*) echo m68k-atari-mint${UNAME_RELEASE} exit ;; milan*:*MiNT:*:* | milan*:*mint:*:* | *milan*:*TOS:*:*) echo m68k-milan-mint${UNAME_RELEASE} exit ;; hades*:*MiNT:*:* | hades*:*mint:*:* | *hades*:*TOS:*:*) echo m68k-hades-mint${UNAME_RELEASE} exit ;; *:*MiNT:*:* | *:*mint:*:* | *:*TOS:*:*) echo m68k-unknown-mint${UNAME_RELEASE} exit ;; m68k:machten:*:*) echo m68k-apple-machten${UNAME_RELEASE} exit ;; powerpc:machten:*:*) echo powerpc-apple-machten${UNAME_RELEASE} exit ;; RISC*:Mach:*:*) echo mips-dec-mach_bsd4.3 exit ;; RISC*:ULTRIX:*:*) echo mips-dec-ultrix${UNAME_RELEASE} exit ;; VAX*:ULTRIX*:*:*) echo vax-dec-ultrix${UNAME_RELEASE} exit ;; 2020:CLIX:*:* | 2430:CLIX:*:*) echo clipper-intergraph-clix${UNAME_RELEASE} exit ;; mips:*:*:UMIPS | mips:*:*:RISCos) eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #ifdef __cplusplus #include <stdio.h> /* for printf() prototype */ int main (int argc, char *argv[]) { #else int main (argc, argv) int argc; char *argv[]; { #endif #if defined (host_mips) && defined (MIPSEB) #if defined (SYSTYPE_SYSV) printf ("mips-mips-riscos%ssysv\n", argv[1]); exit (0); #endif #if defined (SYSTYPE_SVR4) printf ("mips-mips-riscos%ssvr4\n", argv[1]); exit (0); #endif #if defined (SYSTYPE_BSD43) || defined(SYSTYPE_BSD) printf ("mips-mips-riscos%sbsd\n", argv[1]); exit (0); #endif #endif exit (-1); } EOF $CC_FOR_BUILD -o $dummy $dummy.c && dummyarg=`echo "${UNAME_RELEASE}" | sed -n 's/\([0-9]*\).*/\1/p'` && SYSTEM_NAME=`$dummy $dummyarg` && { echo "$SYSTEM_NAME"; exit; } echo mips-mips-riscos${UNAME_RELEASE} exit ;; Motorola:PowerMAX_OS:*:*) echo powerpc-motorola-powermax exit ;; Motorola:*:4.3:PL8-*) echo powerpc-harris-powermax exit ;; Night_Hawk:*:*:PowerMAX_OS | Synergy:PowerMAX_OS:*:*) echo powerpc-harris-powermax exit ;; Night_Hawk:Power_UNIX:*:*) echo powerpc-harris-powerunix exit ;; m88k:CX/UX:7*:*) echo m88k-harris-cxux7 exit ;; m88k:*:4*:R4*) echo m88k-motorola-sysv4 exit ;; m88k:*:3*:R3*) echo m88k-motorola-sysv3 exit ;; AViiON:dgux:*:*) # DG/UX returns AViiON for all architectures UNAME_PROCESSOR=`/usr/bin/uname -p` if [ $UNAME_PROCESSOR = mc88100 ] || [ $UNAME_PROCESSOR = mc88110 ] then if [ ${TARGET_BINARY_INTERFACE}x = m88kdguxelfx ] || \ [ ${TARGET_BINARY_INTERFACE}x = x ] then echo m88k-dg-dgux${UNAME_RELEASE} else echo m88k-dg-dguxbcs${UNAME_RELEASE} fi else echo i586-dg-dgux${UNAME_RELEASE} fi exit ;; M88*:DolphinOS:*:*) # DolphinOS (SVR3) echo m88k-dolphin-sysv3 exit ;; M88*:*:R3*:*) # Delta 88k system running SVR3 echo m88k-motorola-sysv3 exit ;; XD88*:*:*:*) # Tektronix XD88 system running UTekV (SVR3) echo m88k-tektronix-sysv3 exit ;; Tek43[0-9][0-9]:UTek:*:*) # Tektronix 4300 system running UTek (BSD) echo m68k-tektronix-bsd exit ;; *:IRIX*:*:*) echo mips-sgi-irix`echo ${UNAME_RELEASE}|sed -e 's/-/_/g'` exit ;; ????????:AIX?:[12].1:2) # AIX 2.2.1 or AIX 2.1.1 is RT/PC AIX. echo romp-ibm-aix # uname -m gives an 8 hex-code CPU id exit ;; # Note that: echo "'`uname -s`'" gives 'AIX ' i*86:AIX:*:*) echo i386-ibm-aix exit ;; ia64:AIX:*:*) if [ -x /usr/bin/oslevel ] ; then IBM_REV=`/usr/bin/oslevel` else IBM_REV=${UNAME_VERSION}.${UNAME_RELEASE} fi echo ${UNAME_MACHINE}-ibm-aix${IBM_REV} exit ;; *:AIX:2:3) if grep bos325 /usr/include/stdio.h >/dev/null 2>&1; then eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #include <sys/systemcfg.h> main() { if (!__power_pc()) exit(1); puts("powerpc-ibm-aix3.2.5"); exit(0); } EOF if $CC_FOR_BUILD -o $dummy $dummy.c && SYSTEM_NAME=`$dummy` then echo "$SYSTEM_NAME" else echo rs6000-ibm-aix3.2.5 fi elif grep bos324 /usr/include/stdio.h >/dev/null 2>&1; then echo rs6000-ibm-aix3.2.4 else echo rs6000-ibm-aix3.2 fi exit ;; *:AIX:*:[4567]) IBM_CPU_ID=`/usr/sbin/lsdev -C -c processor -S available | sed 1q | awk '{ print $1 }'` if /usr/sbin/lsattr -El ${IBM_CPU_ID} | grep ' POWER' >/dev/null 2>&1; then IBM_ARCH=rs6000 else IBM_ARCH=powerpc fi if [ -x /usr/bin/lslpp ] ; then IBM_REV=`/usr/bin/lslpp -Lqc bos.rte.libc | awk -F: '{ print $3 }' | sed s/[0-9]*$/0/` else IBM_REV=${UNAME_VERSION}.${UNAME_RELEASE} fi echo ${IBM_ARCH}-ibm-aix${IBM_REV} exit ;; *:AIX:*:*) echo rs6000-ibm-aix exit ;; ibmrt:4.4BSD:*|romp-ibm:BSD:*) echo romp-ibm-bsd4.4 exit ;; ibmrt:*BSD:*|romp-ibm:BSD:*) # covers RT/PC BSD and echo romp-ibm-bsd${UNAME_RELEASE} # 4.3 with uname added to exit ;; # report: romp-ibm BSD 4.3 *:BOSX:*:*) echo rs6000-bull-bosx exit ;; DPX/2?00:B.O.S.:*:*) echo m68k-bull-sysv3 exit ;; 9000/[34]??:4.3bsd:1.*:*) echo m68k-hp-bsd exit ;; hp300:4.4BSD:*:* | 9000/[34]??:4.3bsd:2.*:*) echo m68k-hp-bsd4.4 exit ;; 9000/[34678]??:HP-UX:*:*) HPUX_REV=`echo ${UNAME_RELEASE}|sed -e 's/[^.]*.[0B]*//'` case "${UNAME_MACHINE}" in 9000/31? ) HP_ARCH=m68000 ;; 9000/[34]?? ) HP_ARCH=m68k ;; 9000/[678][0-9][0-9]) if [ -x /usr/bin/getconf ]; then sc_cpu_version=`/usr/bin/getconf SC_CPU_VERSION 2>/dev/null` sc_kernel_bits=`/usr/bin/getconf SC_KERNEL_BITS 2>/dev/null` case "${sc_cpu_version}" in 523) HP_ARCH=hppa1.0 ;; # CPU_PA_RISC1_0 528) HP_ARCH=hppa1.1 ;; # CPU_PA_RISC1_1 532) # CPU_PA_RISC2_0 case "${sc_kernel_bits}" in 32) HP_ARCH=hppa2.0n ;; 64) HP_ARCH=hppa2.0w ;; '') HP_ARCH=hppa2.0 ;; # HP-UX 10.20 esac ;; esac fi if [ "${HP_ARCH}" = "" ]; then eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #define _HPUX_SOURCE #include <stdlib.h> #include <unistd.h> int main () { #if defined(_SC_KERNEL_BITS) long bits = sysconf(_SC_KERNEL_BITS); #endif long cpu = sysconf (_SC_CPU_VERSION); switch (cpu) { case CPU_PA_RISC1_0: puts ("hppa1.0"); break; case CPU_PA_RISC1_1: puts ("hppa1.1"); break; case CPU_PA_RISC2_0: #if defined(_SC_KERNEL_BITS) switch (bits) { case 64: puts ("hppa2.0w"); break; case 32: puts ("hppa2.0n"); break; default: puts ("hppa2.0"); break; } break; #else /* !defined(_SC_KERNEL_BITS) */ puts ("hppa2.0"); break; #endif default: puts ("hppa1.0"); break; } exit (0); } EOF (CCOPTS="" $CC_FOR_BUILD -o $dummy $dummy.c 2>/dev/null) && HP_ARCH=`$dummy` test -z "$HP_ARCH" && HP_ARCH=hppa fi ;; esac if [ ${HP_ARCH} = hppa2.0w ] then eval $set_cc_for_build # hppa2.0w-hp-hpux* has a 64-bit kernel and a compiler generating # 32-bit code. hppa64-hp-hpux* has the same kernel and a compiler # generating 64-bit code. GNU and HP use different nomenclature: # # $ CC_FOR_BUILD=cc ./config.guess # => hppa2.0w-hp-hpux11.23 # $ CC_FOR_BUILD="cc +DA2.0w" ./config.guess # => hppa64-hp-hpux11.23 if echo __LP64__ | (CCOPTS="" $CC_FOR_BUILD -E - 2>/dev/null) | grep -q __LP64__ then HP_ARCH=hppa2.0w else HP_ARCH=hppa64 fi fi echo ${HP_ARCH}-hp-hpux${HPUX_REV} exit ;; ia64:HP-UX:*:*) HPUX_REV=`echo ${UNAME_RELEASE}|sed -e 's/[^.]*.[0B]*//'` echo ia64-hp-hpux${HPUX_REV} exit ;; 3050*:HI-UX:*:*) eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #include <unistd.h> int main () { long cpu = sysconf (_SC_CPU_VERSION); /* The order matters, because CPU_IS_HP_MC68K erroneously returns true for CPU_PA_RISC1_0. CPU_IS_PA_RISC returns correct results, however. */ if (CPU_IS_PA_RISC (cpu)) { switch (cpu) { case CPU_PA_RISC1_0: puts ("hppa1.0-hitachi-hiuxwe2"); break; case CPU_PA_RISC1_1: puts ("hppa1.1-hitachi-hiuxwe2"); break; case CPU_PA_RISC2_0: puts ("hppa2.0-hitachi-hiuxwe2"); break; default: puts ("hppa-hitachi-hiuxwe2"); break; } } else if (CPU_IS_HP_MC68K (cpu)) puts ("m68k-hitachi-hiuxwe2"); else puts ("unknown-hitachi-hiuxwe2"); exit (0); } EOF $CC_FOR_BUILD -o $dummy $dummy.c && SYSTEM_NAME=`$dummy` && { echo "$SYSTEM_NAME"; exit; } echo unknown-hitachi-hiuxwe2 exit ;; 9000/7??:4.3bsd:*:* | 9000/8?[79]:4.3bsd:*:* ) echo hppa1.1-hp-bsd exit ;; 9000/8??:4.3bsd:*:*) echo hppa1.0-hp-bsd exit ;; *9??*:MPE/iX:*:* | *3000*:MPE/iX:*:*) echo hppa1.0-hp-mpeix exit ;; hp7??:OSF1:*:* | hp8?[79]:OSF1:*:* ) echo hppa1.1-hp-osf exit ;; hp8??:OSF1:*:*) echo hppa1.0-hp-osf exit ;; i*86:OSF1:*:*) if [ -x /usr/sbin/sysversion ] ; then echo ${UNAME_MACHINE}-unknown-osf1mk else echo ${UNAME_MACHINE}-unknown-osf1 fi exit ;; parisc*:Lites*:*:*) echo hppa1.1-hp-lites exit ;; C1*:ConvexOS:*:* | convex:ConvexOS:C1*:*) echo c1-convex-bsd exit ;; C2*:ConvexOS:*:* | convex:ConvexOS:C2*:*) if getsysinfo -f scalar_acc then echo c32-convex-bsd else echo c2-convex-bsd fi exit ;; C34*:ConvexOS:*:* | convex:ConvexOS:C34*:*) echo c34-convex-bsd exit ;; C38*:ConvexOS:*:* | convex:ConvexOS:C38*:*) echo c38-convex-bsd exit ;; C4*:ConvexOS:*:* | convex:ConvexOS:C4*:*) echo c4-convex-bsd exit ;; CRAY*Y-MP:*:*:*) echo ymp-cray-unicos${UNAME_RELEASE} | sed -e 's/\.[^.]*$/.X/' exit ;; CRAY*[A-Z]90:*:*:*) echo ${UNAME_MACHINE}-cray-unicos${UNAME_RELEASE} \ | sed -e 's/CRAY.*\([A-Z]90\)/\1/' \ -e y/ABCDEFGHIJKLMNOPQRSTUVWXYZ/abcdefghijklmnopqrstuvwxyz/ \ -e 's/\.[^.]*$/.X/' exit ;; CRAY*TS:*:*:*) echo t90-cray-unicos${UNAME_RELEASE} | sed -e 's/\.[^.]*$/.X/' exit ;; CRAY*T3E:*:*:*) echo alphaev5-cray-unicosmk${UNAME_RELEASE} | sed -e 's/\.[^.]*$/.X/' exit ;; CRAY*SV1:*:*:*) echo sv1-cray-unicos${UNAME_RELEASE} | sed -e 's/\.[^.]*$/.X/' exit ;; *:UNICOS/mp:*:*) echo craynv-cray-unicosmp${UNAME_RELEASE} | sed -e 's/\.[^.]*$/.X/' exit ;; F30[01]:UNIX_System_V:*:* | F700:UNIX_System_V:*:*) FUJITSU_PROC=`uname -m | tr ABCDEFGHIJKLMNOPQRSTUVWXYZ abcdefghijklmnopqrstuvwxyz` FUJITSU_SYS=`uname -p | tr ABCDEFGHIJKLMNOPQRSTUVWXYZ abcdefghijklmnopqrstuvwxyz | sed -e 's/\///'` FUJITSU_REL=`echo ${UNAME_RELEASE} | sed -e 's/ /_/'` echo "${FUJITSU_PROC}-fujitsu-${FUJITSU_SYS}${FUJITSU_REL}" exit ;; 5000:UNIX_System_V:4.*:*) FUJITSU_SYS=`uname -p | tr ABCDEFGHIJKLMNOPQRSTUVWXYZ abcdefghijklmnopqrstuvwxyz | sed -e 's/\///'` FUJITSU_REL=`echo ${UNAME_RELEASE} | tr ABCDEFGHIJKLMNOPQRSTUVWXYZ abcdefghijklmnopqrstuvwxyz | sed -e 's/ /_/'` echo "sparc-fujitsu-${FUJITSU_SYS}${FUJITSU_REL}" exit ;; i*86:BSD/386:*:* | i*86:BSD/OS:*:* | *:Ascend\ Embedded/OS:*:*) echo ${UNAME_MACHINE}-pc-bsdi${UNAME_RELEASE} exit ;; sparc*:BSD/OS:*:*) echo sparc-unknown-bsdi${UNAME_RELEASE} exit ;; *:BSD/OS:*:*) echo ${UNAME_MACHINE}-unknown-bsdi${UNAME_RELEASE} exit ;; *:FreeBSD:*:*) UNAME_PROCESSOR=`/usr/bin/uname -p` case ${UNAME_PROCESSOR} in amd64) echo x86_64-unknown-freebsd`echo ${UNAME_RELEASE}|sed -e 's/[-(].*//'` ;; *) echo ${UNAME_PROCESSOR}-unknown-freebsd`echo ${UNAME_RELEASE}|sed -e 's/[-(].*//'` ;; esac exit ;; i*:CYGWIN*:*) echo ${UNAME_MACHINE}-pc-cygwin exit ;; *:MINGW64*:*) echo ${UNAME_MACHINE}-pc-mingw64 exit ;; *:MINGW*:*) echo ${UNAME_MACHINE}-pc-mingw32 exit ;; *:MSYS*:*) echo ${UNAME_MACHINE}-pc-msys exit ;; i*:windows32*:*) # uname -m includes "-pc" on this system. echo ${UNAME_MACHINE}-mingw32 exit ;; i*:PW*:*) echo ${UNAME_MACHINE}-pc-pw32 exit ;; *:Interix*:*) case ${UNAME_MACHINE} in x86) echo i586-pc-interix${UNAME_RELEASE} exit ;; authenticamd | genuineintel | EM64T) echo x86_64-unknown-interix${UNAME_RELEASE} exit ;; IA64) echo ia64-unknown-interix${UNAME_RELEASE} exit ;; esac ;; [345]86:Windows_95:* | [345]86:Windows_98:* | [345]86:Windows_NT:*) echo i${UNAME_MACHINE}-pc-mks exit ;; 8664:Windows_NT:*) echo x86_64-pc-mks exit ;; i*:Windows_NT*:* | Pentium*:Windows_NT*:*) # How do we know it's Interix rather than the generic POSIX subsystem? # It also conflicts with pre-2.0 versions of AT&T UWIN. Should we # UNAME_MACHINE based on the output of uname instead of i386? echo i586-pc-interix exit ;; i*:UWIN*:*) echo ${UNAME_MACHINE}-pc-uwin exit ;; amd64:CYGWIN*:*:* | x86_64:CYGWIN*:*:*) echo x86_64-unknown-cygwin exit ;; p*:CYGWIN*:*) echo powerpcle-unknown-cygwin exit ;; prep*:SunOS:5.*:*) echo powerpcle-unknown-solaris2`echo ${UNAME_RELEASE}|sed -e 's/[^.]*//'` exit ;; *:GNU:*:*) # the GNU system echo `echo ${UNAME_MACHINE}|sed -e 's,[-/].*$,,'`-unknown-${LIBC}`echo ${UNAME_RELEASE}|sed -e 's,/.*$,,'` exit ;; *:GNU/*:*:*) # other systems with GNU libc and userland echo ${UNAME_MACHINE}-unknown-`echo ${UNAME_SYSTEM} | sed 's,^[^/]*/,,' | tr "[:upper:]" "[:lower:]"``echo ${UNAME_RELEASE}|sed -e 's/[-(].*//'`-${LIBC} exit ;; i*86:Minix:*:*) echo ${UNAME_MACHINE}-pc-minix exit ;; aarch64:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; aarch64_be:Linux:*:*) UNAME_MACHINE=aarch64_be echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; alpha:Linux:*:*) case `sed -n '/^cpu model/s/^.*: \(.*\)/\1/p' < /proc/cpuinfo` in EV5) UNAME_MACHINE=alphaev5 ;; EV56) UNAME_MACHINE=alphaev56 ;; PCA56) UNAME_MACHINE=alphapca56 ;; PCA57) UNAME_MACHINE=alphapca56 ;; EV6) UNAME_MACHINE=alphaev6 ;; EV67) UNAME_MACHINE=alphaev67 ;; EV68*) UNAME_MACHINE=alphaev68 ;; esac objdump --private-headers /bin/sh | grep -q ld.so.1 if test "$?" = 0 ; then LIBC=gnulibc1 ; fi echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; arc:Linux:*:* | arceb:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; arm*:Linux:*:*) eval $set_cc_for_build if echo __ARM_EABI__ | $CC_FOR_BUILD -E - 2>/dev/null \ | grep -q __ARM_EABI__ then echo ${UNAME_MACHINE}-unknown-linux-${LIBC} else if echo __ARM_PCS_VFP | $CC_FOR_BUILD -E - 2>/dev/null \ | grep -q __ARM_PCS_VFP then echo ${UNAME_MACHINE}-unknown-linux-${LIBC}eabi else echo ${UNAME_MACHINE}-unknown-linux-${LIBC}eabihf fi fi exit ;; avr32*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; cris:Linux:*:*) echo ${UNAME_MACHINE}-axis-linux-${LIBC} exit ;; crisv32:Linux:*:*) echo ${UNAME_MACHINE}-axis-linux-${LIBC} exit ;; e2k:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; frv:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; hexagon:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; i*86:Linux:*:*) echo ${UNAME_MACHINE}-pc-linux-${LIBC} exit ;; ia64:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; k1om:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; m32r*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; m68*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; mips:Linux:*:* | mips64:Linux:*:*) eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #undef CPU #undef ${UNAME_MACHINE} #undef ${UNAME_MACHINE}el #if defined(__MIPSEL__) || defined(__MIPSEL) || defined(_MIPSEL) || defined(MIPSEL) CPU=${UNAME_MACHINE}el #else #if defined(__MIPSEB__) || defined(__MIPSEB) || defined(_MIPSEB) || defined(MIPSEB) CPU=${UNAME_MACHINE} #else CPU= #endif #endif EOF eval `$CC_FOR_BUILD -E $dummy.c 2>/dev/null | grep '^CPU'` test x"${CPU}" != x && { echo "${CPU}-unknown-linux-${LIBC}"; exit; } ;; mips64el:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; openrisc*:Linux:*:*) echo or1k-unknown-linux-${LIBC} exit ;; or32:Linux:*:* | or1k*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; padre:Linux:*:*) echo sparc-unknown-linux-${LIBC} exit ;; parisc64:Linux:*:* | hppa64:Linux:*:*) echo hppa64-unknown-linux-${LIBC} exit ;; parisc:Linux:*:* | hppa:Linux:*:*) # Look for CPU level case `grep '^cpu[^a-z]*:' /proc/cpuinfo 2>/dev/null | cut -d' ' -f2` in PA7*) echo hppa1.1-unknown-linux-${LIBC} ;; PA8*) echo hppa2.0-unknown-linux-${LIBC} ;; *) echo hppa-unknown-linux-${LIBC} ;; esac exit ;; ppc64:Linux:*:*) echo powerpc64-unknown-linux-${LIBC} exit ;; ppc:Linux:*:*) echo powerpc-unknown-linux-${LIBC} exit ;; ppc64le:Linux:*:*) echo powerpc64le-unknown-linux-${LIBC} exit ;; ppcle:Linux:*:*) echo powerpcle-unknown-linux-${LIBC} exit ;; riscv32:Linux:*:* | riscv64:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; s390:Linux:*:* | s390x:Linux:*:*) echo ${UNAME_MACHINE}-ibm-linux-${LIBC} exit ;; sh64*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; sh*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; sparc:Linux:*:* | sparc64:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; tile*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; vax:Linux:*:*) echo ${UNAME_MACHINE}-dec-linux-${LIBC} exit ;; x86_64:Linux:*:*) echo ${UNAME_MACHINE}-pc-linux-${LIBC} exit ;; xtensa*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; i*86:DYNIX/ptx:4*:*) # ptx 4.0 does uname -s correctly, with DYNIX/ptx in there. # earlier versions are messed up and put the nodename in both # sysname and nodename. echo i386-sequent-sysv4 exit ;; i*86:UNIX_SV:4.2MP:2.*) # Unixware is an offshoot of SVR4, but it has its own version # number series starting with 2... # I am not positive that other SVR4 systems won't match this, # I just have to hope. -- rms. # Use sysv4.2uw... so that sysv4* matches it. echo ${UNAME_MACHINE}-pc-sysv4.2uw${UNAME_VERSION} exit ;; i*86:OS/2:*:*) # If we were able to find `uname', then EMX Unix compatibility # is probably installed. echo ${UNAME_MACHINE}-pc-os2-emx exit ;; i*86:XTS-300:*:STOP) echo ${UNAME_MACHINE}-unknown-stop exit ;; i*86:atheos:*:*) echo ${UNAME_MACHINE}-unknown-atheos exit ;; i*86:syllable:*:*) echo ${UNAME_MACHINE}-pc-syllable exit ;; i*86:LynxOS:2.*:* | i*86:LynxOS:3.[01]*:* | i*86:LynxOS:4.[02]*:*) echo i386-unknown-lynxos${UNAME_RELEASE} exit ;; i*86:*DOS:*:*) echo ${UNAME_MACHINE}-pc-msdosdjgpp exit ;; i*86:*:4.*:* | i*86:SYSTEM_V:4.*:*) UNAME_REL=`echo ${UNAME_RELEASE} | sed 's/\/MP$//'` if grep Novell /usr/include/link.h >/dev/null 2>/dev/null; then echo ${UNAME_MACHINE}-univel-sysv${UNAME_REL} else echo ${UNAME_MACHINE}-pc-sysv${UNAME_REL} fi exit ;; i*86:*:5:[678]*) # UnixWare 7.x, OpenUNIX and OpenServer 6. case `/bin/uname -X | grep "^Machine"` in *486*) UNAME_MACHINE=i486 ;; *Pentium) UNAME_MACHINE=i586 ;; *Pent*|*Celeron) UNAME_MACHINE=i686 ;; esac echo ${UNAME_MACHINE}-unknown-sysv${UNAME_RELEASE}${UNAME_SYSTEM}${UNAME_VERSION} exit ;; i*86:*:3.2:*) if test -f /usr/options/cb.name; then UNAME_REL=`sed -n 's/.*Version //p' </usr/options/cb.name` echo ${UNAME_MACHINE}-pc-isc$UNAME_REL elif /bin/uname -X 2>/dev/null >/dev/null ; then UNAME_REL=`(/bin/uname -X|grep Release|sed -e 's/.*= //')` (/bin/uname -X|grep i80486 >/dev/null) && UNAME_MACHINE=i486 (/bin/uname -X|grep '^Machine.*Pentium' >/dev/null) \ && UNAME_MACHINE=i586 (/bin/uname -X|grep '^Machine.*Pent *II' >/dev/null) \ && UNAME_MACHINE=i686 (/bin/uname -X|grep '^Machine.*Pentium Pro' >/dev/null) \ && UNAME_MACHINE=i686 echo ${UNAME_MACHINE}-pc-sco$UNAME_REL else echo ${UNAME_MACHINE}-pc-sysv32 fi exit ;; pc:*:*:*) # Left here for compatibility: # uname -m prints for DJGPP always 'pc', but it prints nothing about # the processor, so we play safe by assuming i586. # Note: whatever this is, it MUST be the same as what config.sub # prints for the "djgpp" host, or else GDB configure will decide that # this is a cross-build. echo i586-pc-msdosdjgpp exit ;; Intel:Mach:3*:*) echo i386-pc-mach3 exit ;; paragon:*:*:*) echo i860-intel-osf1 exit ;; i860:*:4.*:*) # i860-SVR4 if grep Stardent /usr/include/sys/uadmin.h >/dev/null 2>&1 ; then echo i860-stardent-sysv${UNAME_RELEASE} # Stardent Vistra i860-SVR4 else # Add other i860-SVR4 vendors below as they are discovered. echo i860-unknown-sysv${UNAME_RELEASE} # Unknown i860-SVR4 fi exit ;; mini*:CTIX:SYS*5:*) # "miniframe" echo m68010-convergent-sysv exit ;; mc68k:UNIX:SYSTEM5:3.51m) echo m68k-convergent-sysv exit ;; M680?0:D-NIX:5.3:*) echo m68k-diab-dnix exit ;; M68*:*:R3V[5678]*:*) test -r /sysV68 && { echo 'm68k-motorola-sysv'; exit; } ;; 3[345]??:*:4.0:3.0 | 3[34]??A:*:4.0:3.0 | 3[34]??,*:*:4.0:3.0 | 3[34]??/*:*:4.0:3.0 | 4400:*:4.0:3.0 | 4850:*:4.0:3.0 | SKA40:*:4.0:3.0 | SDS2:*:4.0:3.0 | SHG2:*:4.0:3.0 | S7501*:*:4.0:3.0) OS_REL='' test -r /etc/.relid \ && OS_REL=.`sed -n 's/[^ ]* [^ ]* \([0-9][0-9]\).*/\1/p' < /etc/.relid` /bin/uname -p 2>/dev/null | grep 86 >/dev/null \ && { echo i486-ncr-sysv4.3${OS_REL}; exit; } /bin/uname -p 2>/dev/null | /bin/grep entium >/dev/null \ && { echo i586-ncr-sysv4.3${OS_REL}; exit; } ;; 3[34]??:*:4.0:* | 3[34]??,*:*:4.0:*) /bin/uname -p 2>/dev/null | grep 86 >/dev/null \ && { echo i486-ncr-sysv4; exit; } ;; NCR*:*:4.2:* | MPRAS*:*:4.2:*) OS_REL='.3' test -r /etc/.relid \ && OS_REL=.`sed -n 's/[^ ]* [^ ]* \([0-9][0-9]\).*/\1/p' < /etc/.relid` /bin/uname -p 2>/dev/null | grep 86 >/dev/null \ && { echo i486-ncr-sysv4.3${OS_REL}; exit; } /bin/uname -p 2>/dev/null | /bin/grep entium >/dev/null \ && { echo i586-ncr-sysv4.3${OS_REL}; exit; } /bin/uname -p 2>/dev/null | /bin/grep pteron >/dev/null \ && { echo i586-ncr-sysv4.3${OS_REL}; exit; } ;; m68*:LynxOS:2.*:* | m68*:LynxOS:3.0*:*) echo m68k-unknown-lynxos${UNAME_RELEASE} exit ;; mc68030:UNIX_System_V:4.*:*) echo m68k-atari-sysv4 exit ;; TSUNAMI:LynxOS:2.*:*) echo sparc-unknown-lynxos${UNAME_RELEASE} exit ;; rs6000:LynxOS:2.*:*) echo rs6000-unknown-lynxos${UNAME_RELEASE} exit ;; PowerPC:LynxOS:2.*:* | PowerPC:LynxOS:3.[01]*:* | PowerPC:LynxOS:4.[02]*:*) echo powerpc-unknown-lynxos${UNAME_RELEASE} exit ;; SM[BE]S:UNIX_SV:*:*) echo mips-dde-sysv${UNAME_RELEASE} exit ;; RM*:ReliantUNIX-*:*:*) echo mips-sni-sysv4 exit ;; RM*:SINIX-*:*:*) echo mips-sni-sysv4 exit ;; *:SINIX-*:*:*) if uname -p 2>/dev/null >/dev/null ; then UNAME_MACHINE=`(uname -p) 2>/dev/null` echo ${UNAME_MACHINE}-sni-sysv4 else echo ns32k-sni-sysv fi exit ;; PENTIUM:*:4.0*:*) # Unisys `ClearPath HMP IX 4000' SVR4/MP effort # says <Richard.M.Bartel@ccMail.Census.GOV> echo i586-unisys-sysv4 exit ;; *:UNIX_System_V:4*:FTX*) # From Gerald Hewes <hewes@openmarket.com>. # How about differentiating between stratus architectures? -djm echo hppa1.1-stratus-sysv4 exit ;; *:*:*:FTX*) # From seanf@swdc.stratus.com. echo i860-stratus-sysv4 exit ;; i*86:VOS:*:*) # From Paul.Green@stratus.com. echo ${UNAME_MACHINE}-stratus-vos exit ;; *:VOS:*:*) # From Paul.Green@stratus.com. echo hppa1.1-stratus-vos exit ;; mc68*:A/UX:*:*) echo m68k-apple-aux${UNAME_RELEASE} exit ;; news*:NEWS-OS:6*:*) echo mips-sony-newsos6 exit ;; R[34]000:*System_V*:*:* | R4000:UNIX_SYSV:*:* | R*000:UNIX_SV:*:*) if [ -d /usr/nec ]; then echo mips-nec-sysv${UNAME_RELEASE} else echo mips-unknown-sysv${UNAME_RELEASE} fi exit ;; BeBox:BeOS:*:*) # BeOS running on hardware made by Be, PPC only. echo powerpc-be-beos exit ;; BeMac:BeOS:*:*) # BeOS running on Mac or Mac clone, PPC only. echo powerpc-apple-beos exit ;; BePC:BeOS:*:*) # BeOS running on Intel PC compatible. echo i586-pc-beos exit ;; BePC:Haiku:*:*) # Haiku running on Intel PC compatible. echo i586-pc-haiku exit ;; x86_64:Haiku:*:*) echo x86_64-unknown-haiku exit ;; SX-4:SUPER-UX:*:*) echo sx4-nec-superux${UNAME_RELEASE} exit ;; SX-5:SUPER-UX:*:*) echo sx5-nec-superux${UNAME_RELEASE} exit ;; SX-6:SUPER-UX:*:*) echo sx6-nec-superux${UNAME_RELEASE} exit ;; SX-7:SUPER-UX:*:*) echo sx7-nec-superux${UNAME_RELEASE} exit ;; SX-8:SUPER-UX:*:*) echo sx8-nec-superux${UNAME_RELEASE} exit ;; SX-8R:SUPER-UX:*:*) echo sx8r-nec-superux${UNAME_RELEASE} exit ;; SX-ACE:SUPER-UX:*:*) echo sxace-nec-superux${UNAME_RELEASE} exit ;; Power*:Rhapsody:*:*) echo powerpc-apple-rhapsody${UNAME_RELEASE} exit ;; 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See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see <http://www.gnu.org/licenses/>. # As a special exception to the GNU General Public License, if you # distribute this file as part of a program that contains a # configuration script generated by Autoconf, you may include it under # the same distribution terms that you use for the rest of that program. # This file is maintained in Automake, please report # bugs to <bug-automake@gnu.org> or send patches to # <automake-patches@gnu.org>. # func_error message func_error () { echo "$me: $1" 1>&2 exit 1 } file_conv= # func_file_conv build_file # Convert a $build file to $host form and store it in $file # Currently only supports Windows hosts. func_file_conv () { file=$1 case $file in / | /[!/]*) # absolute file, and not a UNC file if test -z "$file_conv"; then # lazily determine how to convert abs files case `uname -s` in MINGW*) file_conv=mingw ;; CYGWIN*) file_conv=cygwin ;; *) file_conv=wine ;; esac fi case $file_conv in mingw) file=`cmd //C echo "$file " | sed -e 's/"\(.*\) " *$/\1/'` ;; cygwin) file=`cygpath -m "$file" || echo "$file"` ;; wine) file=`winepath -w "$file" || echo "$file"` ;; esac ;; esac } # func_at_file at_file operation archive # Iterate over all members in AT_FILE performing OPERATION on ARCHIVE # for each of them. # When interpreting the content of the @FILE, do NOT use func_file_conv, # since the user would need to supply preconverted file names to # binutils ar, at least for MinGW. func_at_file () { operation=$2 archive=$3 at_file_contents=`cat "$1"` eval set x "$at_file_contents" shift for member do $AR -NOLOGO $operation:"$member" "$archive" || exit $? done } case $1 in '') func_error "no command. 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specified" ;; esac action=${action#?} done case $delete$extract$list$quick$replace,$index in yes,* | ,yes) ;; yesyes*) func_error "more than one action specified" ;; *) func_error "no action specified" ;; esac if test -n "$delete"; then if test ! -f "$orig_archive"; then func_error "archive not found" fi for member do case $1 in @*) func_at_file "${1#@}" -REMOVE "$archive" ;; *) func_file_conv "$1" $AR -NOLOGO -REMOVE:"$file" "$archive" || exit $? ;; esac done elif test -n "$extract"; then if test ! -f "$orig_archive"; then func_error "archive not found" fi if test $# -gt 0; then for member do case $1 in @*) func_at_file "${1#@}" -EXTRACT "$archive" ;; *) func_file_conv "$1" $AR -NOLOGO -EXTRACT:"$file" "$archive" || exit $? ;; esac done else $AR -NOLOGO -LIST "$archive" | sed -e 's/\\/\\\\/g' | while read member do $AR -NOLOGO -EXTRACT:"$member" "$archive" || exit $? done fi elif test -n "$quick$replace"; then if test ! -f "$orig_archive"; then if test -z "$create"; then echo "$me: creating $orig_archive" fi orig_archive= else orig_archive=$archive fi for member do case $1 in @*) func_file_conv "${1#@}" set x "$@" "@$file" ;; *) func_file_conv "$1" set x "$@" "$file" ;; esac shift shift done if test -n "$orig_archive"; then $AR -NOLOGO -OUT:"$archive" "$orig_archive" "$@" || exit $? else $AR -NOLOGO -OUT:"$archive" "$@" || exit $? fi elif test -n "$list"; then if test ! -f "$orig_archive"; then func_error "archive not found" fi $AR -NOLOGO -LIST "$archive" || exit $? fi 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