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#!/bin/sh
#
# Wrapper script used to calculate the luminosity (Lx) and flux (Fx) data,
# which invokes the programming 'calc_lx_beta' (single-beta SBP) or
# 'calc_lx_dbeta' (double-beta SBP).
#
# Output:
# * lx_result.txt
# * fx_result.txt
# * summary_lx.dat
# * summary_fx.dat
# * lx_beta_param.txt / lx_dbeta_param.txt
#
# Author: Junhua GU
# Created: 2013-06-24
#
# Weitian LI
# 2016-06-07
#
if [ $# -eq 2 ] || [ $# -eq 3 ]; then
:
else
echo "usage:"
echo " `basename $0` <global.cfg> <rout_kpc> [c]"
echo ""
echo "arguments:"
echo " <global.cfg>: main config file used for mass calculation"
echo " <rout_kpc>: outer/cut radius within which to calculate Lx & Fx"
echo " e.g., r500, r200 (unit: kpc)"
echo " [c]: optional; if specified, do not calculate the errors"
exit 1
fi
export PATH="/usr/local/bin:/usr/bin:/bin:$PATH"
export PGPLOT_FONT="${HEADAS}/lib/grfont.dat"
cfg_file="$1"
rout="$2"
case "$3" in
[cC])
F_C="YES"
;;
*)
F_C="NO"
;;
esac
base_path=$(dirname $(realpath $0))
## Extract settings/values from the config file
# model name of the temperature profile
t_profile_type=`grep '^t_profile' $cfg_file | awk '{ print $2 }'`
# parameter file for temperature profile fitting
t_param_file=`grep '^t_param_file' $cfg_file | awk '{ print $2 }'`
# data points of the temperature profile
t_data_file=`grep '^t_data_file' $cfg_file | awk '{ print $2 }'`
# config file for SBP fitting
sbp_cfg=`grep '^sbp_cfg' $cfg_file | awk '{ print $2 }'`
# SBP flux data
sbp_data_file=`grep '^sbp_file' $sbp_cfg | awk '{ print $2 }'`
# fitted temperature profile
T_file=`grep '^T_file' $sbp_cfg | awk '{ print $2 }'`
# filename of the cooling function data
cfunc_file=`grep '^cfunc_file' $sbp_cfg |awk '{ print $2 }'`
nfw_rmin_kpc=`grep '^nfw_rmin_kpc' $cfg_file | awk '{ print $2 }'`
cm_per_pixel=`grep '^cm_per_pixel' $sbp_cfg | awk '{ print $2 }'`
z=`grep '^z' $sbp_cfg | awk '{ print $2 }'`
nh=`grep '^nh' $cfg_file |awk '{ print $2 }'`
abund=`grep '^abund' $cfg_file |awk '{ print $2 }'`
da=`python -c "print($cm_per_pixel/(0.492/3600/180*3.1415926))"`
dl=`python -c "print($da*(1+$z)**2)"`
if grep -q '^beta2' $sbp_cfg; then
MODEL="dbeta"
else
MODEL="beta"
fi
if [ "$t_profile_type" = "wang2012" ]; then
${base_path}/fit_wang2012_model $t_data_file $t_param_file $cm_per_pixel 2> /dev/null
mv -f wang2012_dump.qdp ${T_file}
else
echo "ERROR: unsupported temperature profile: ${t_profile_type}"
exit 11
fi
# energy bands for which the cooling function data will be calculated
BLIST="blist.txt"
[ -e "${BLIST}" ] && mv -f ${BLIST} ${BLIST}_bak
cat > ${BLIST} << _EOF_
bolo
0.7 7
0.1 2.4
_EOF_
${base_path}/coolfunc_calc.sh ${T_file} $abund $nh $z $cfunc_file
${base_path}/coolfunc_calc_erg.sh ${T_file} $abund $nh $z "cfunc_" ${BLIST}
mv flux_cnt_ratio.txt flux_cnt_ratio_center.txt
PROG="calc_lx_${MODEL}"
LXF_RES="lx_${MODEL}_param.txt"
${base_path}/${PROG} ${sbp_cfg} ${rout} \
cfunc_bolo.dat \
cfunc_0.7-7.dat \
cfunc_0.1-2.4.dat 2> /dev/null
LX1=`grep '^Lx1' ${LX_RES} | awk '{ print $2 }'`
LX2=`grep '^Lx2' ${LX_RES} | awk '{ print $2 }'`
LX3=`grep '^Lx3' ${LX_RES} | awk '{ print $2 }'`
FX1=`grep '^Fx1' ${LX_RES} | awk '{ print $2 }'`
FX2=`grep '^Fx2' ${LX_RES} | awk '{ print $2 }'`
FX3=`grep '^Fx3' ${LX_RES} | awk '{ print $2 }'`
echo "${LX1} ${LX2} ${LX3}" >summary_lx.dat
echo "${FX1} ${FX2} ${FX3}" >summary_fx.dat
# save the calculated central values
mv ${LX_RES} ${LX_RES%.txt}_center.txt
mv lx_sbp_fit.qdp lx_sbp_fit_center.qdp
mv lx_rho_fit.dat lx_rho_fit_center.dat
# only calculate the central values
if [ "${F_C}" = "YES" ]; then
echo "Calculate the central values only ..."
${base_path}/analyze_lxfx.py "Lx" summary_lx.dat lx_result.txt ${BLIST}
${base_path}/analyze_lxfx.py "Fx" summary_fx.dat fx_result.txt ${BLIST}
exit 0
fi
###########################################################
# Estimate the errors of Lx and Fx by Monte Carlo simulation
MC_TIMES=100
for i in `seq 1 ${MC_TIMES}`; do
$base_path/shuffle_T.py $t_data_file temp_shuffled_t.dat
$base_path/shuffle_sbp.py $sbp_data_file temp_shuffled_sbp.dat
if [ "$t_profile_type" = "wang2012" ]; then
${base_path}/fit_wang2012_model temp_shuffled_t.dat $t_param_file $cm_per_pixel 2> /dev/null
mv -f wang2012_dump.qdp ${T_file}
else
echo "ERROR: unsupported temperature profile: ${t_profile_type}"
exit 11
fi
# clear ${TMP_SBP_CFG}
TMP_SBP_CFG="temp_sbp.cfg"
# : > ${TMP_SBP_CFG}
[ -e "${TMP_SBP_CFG}" ] && rm -f ${TMP_SBP_CFG}
cat ${sbp_cfg} | while read l; do
if echo "${l}" | grep -q '^sbp_file' >/dev/null; then
echo "sbp_file temp_shuffled_sbp.dat" >> ${TMP_SBP_CFG}
elif echo "${l}" | grep -q '^T_file' >/dev/null; then
echo "T_file ${T_file}" >> ${TMP_SBP_CFG}
else
echo "${l}" >> ${TMP_SBP_CFG}
fi
done
echo "### `pwd -P`"
echo "### $i / ${MC_TIMES} ###"
${base_path}/coolfunc_calc.sh ${T_file} $abund $nh $z $cfunc_file
${base_path}/coolfunc_calc_erg.sh ${T_file} $abund $nh $z "cfunc_" ${BLIST}
${base_path}/${PROG} temp_sbp.cfg ${rout} \
cfunc_bolo.dat \
cfunc_0.7-7.dat \
cfunc_0.1-2.4.dat 2> /dev/null
LX1=`grep '^Lx1' ${LX_RES} | awk '{ print $2 }'`
LX2=`grep '^Lx2' ${LX_RES} | awk '{ print $2 }'`
LX3=`grep '^Lx3' ${LX_RES} | awk '{ print $2 }'`
FX1=`grep '^Fx1' ${LX_RES} | awk '{ print $2 }'`
FX2=`grep '^Fx2' ${LX_RES} | awk '{ print $2 }'`
FX3=`grep '^Fx3' ${LX_RES} | awk '{ print $2 }'`
echo "${LX1} ${LX2} ${LX3}" >>summary_lx.dat
echo "${FX1} ${FX2} ${FX3}" >>summary_fx.dat
done # end of 'for'
# analyze Lx & Fx Monte Carlo results
${base_path}/analyze_lxfx.py "Lx" summary_lx.dat lx_result.txt ${BLIST}
${base_path}/analyze_lxfx.py "Fx" summary_fx.dat fx_result.txt ${BLIST}
exit 0
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