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author | Aaron LI <aaronly.me@outlook.com> | 2017-02-21 23:32:51 +0800 |
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committer | Aaron LI <aaronly.me@outlook.com> | 2017-02-21 23:32:51 +0800 |
commit | 361e52204d2bc67b69e1e2a6823da0e95d5a530a (patch) | |
tree | d35d9fe524287d46bd7a07ac7b12d86833508775 /bin | |
parent | 04683a56e493133086193bba2f85ac0f7b5d4a81 (diff) | |
download | chandra-acis-analysis-361e52204d2bc67b69e1e2a6823da0e95d5a530a.tar.bz2 |
Remove calc_coolfunc.sh (replaced by calc_coolfunc_{table,profile}.py)
Diffstat (limited to 'bin')
-rwxr-xr-x | bin/calc_coolfunc.sh | 113 |
1 files changed, 0 insertions, 113 deletions
diff --git a/bin/calc_coolfunc.sh b/bin/calc_coolfunc.sh deleted file mode 100755 index d1d0b35..0000000 --- a/bin/calc_coolfunc.sh +++ /dev/null @@ -1,113 +0,0 @@ -#!/bin/sh -## -## Calculate the 'cooling function' profile with respect to the -## given 'temperature profile' and the average abundance, redshift, -## and column density nH, using the XSPEC model 'wabs*apec'. -## -## NOTE: -## The output cooling function values should be the 'flux' values -## with unit 'photon/s/cm^2' (different to 'calc_coolfunc_bands.sh'). -## These results will be used by 'fit_{beta,dbeta}_sbp' to derive the -## (3D) gas density profile from (2D) surface brightness profile, -## whose values have unit 'photon/cm^2/pixel/s'. -## -## Weitian LI -## Created: 2012-08-17 -## -## Change logs: -## 2017-02-17, Weitian LI -## * Rename from 'coolfunc_calc.sh' to 'calc_coolfunc.sh' -## * Clean up that do not calculate and output <coolfunc_bolo> -## 2017-02-16, Weitian LI -## * Do not calculate and output 'flux_cnt_ratio.txt' -## - -## cmdline arguments {{{ -if [ $# -ne 5 ]; then - printf "usage:\n" - printf " `basename $0` <tprofile> <avg_abund> <nH> <redshift> <coolfunc_outfile>\n" - exit 1 -fi -TPROFILE=$1 -ABUNDANCE=$2 -N_H=$3 -REDSHIFT=$4 -COOLFUNC_DAT=$5 -NORM=`cosmo_calc ${REDSHIFT} | grep 'norm.*cooling_function' | awk -F':' '{ print $2 }'` - -if [ ! -r "${TPROFILE}" ]; then - printf "ERROR: given tprofile '${TPROFILE}' NOT accessiable\n" - exit 2 -fi -[ -e "${COOLFUNC_DAT}" ] && rm -f ${COOLFUNC_DAT} -## arguments }}} - -XSPEC_CF_XCM="_calc_coolfunc.xcm" -[ -e "${XSPEC_CF_XCM}" ] && rm -f ${XSPEC_CF_XCM} - -## generate xspec script {{{ -cat > ${XSPEC_CF_XCM} << _EOF_ -## XSPEC Tcl script -## Calculate the cooling function profile w.r.t the temperature profile. -## -## Generated by: `basename $0` -## Date: `date` - -set xs_return_results 1 -set xs_echo_script 0 -# set tcl_precision 12 -## set basic data {{{ -set nh ${N_H} -set redshift ${REDSHIFT} -set abundance ${ABUNDANCE} -set norm ${NORM} -## basic }}} - -## xspec related {{{ -# debug settings {{{ -chatter 0 -# debug }}} -query yes -abund grsa -dummyrsp 0.01 100.0 4096 linear -# load model 'wabs*apec' to calc cooling function -model wabs*apec & \${nh} & 1.0 & \${abundance} & \${redshift} & \${norm} & /* -## xspec }}} - -## set input and output filename & open files -set tpro_fn "${TPROFILE}" -set cf_fn "${COOLFUNC_DAT}" -if { [ file exists \${cf_fn} ] } { - exec rm -fv \${cf_fn} -} - -## open files -set tpro_fd [ open \${tpro_fn} r ] -set cf_fd [ open \${cf_fn} w ] - -## read data from tprofile line by line -while { [ gets \${tpro_fd} tpro_line ] != -1 } { - scan \${tpro_line} "%f %f" radius temperature - #puts "radius: \${radius}, temperature: \${temperature}" - # set temperature value - newpar 2 \${temperature} - # calc flux & tclout - flux 0.7 7.0 - tclout flux 1 - scan \${xspec_tclout} "%f %f %f %f" _ _ _ cf_photon - #puts "cf: \${cf_photon}" - puts \${cf_fd} "\${radius} \${cf_photon}" -} - -## close opened files -close \${tpro_fd} -close \${cf_fd} - -## exit -tclexit -_EOF_ -## xcm generation }}} - -## invoke xspec to calc -printf "invoking XSPEC to calculate cooling function profile ...\n" -xspec - ${XSPEC_CF_XCM} > /dev/null |