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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 $0` <mass.conf> <rout_kpc> [c]"
echo ""
echo "arguments:"
echo " <mass.conf>: config file for mass profile calculation"
echo " <rout_kpc>: outer/cut radius within which to calculate Lx & Fx"
echo " e.g., r500, r200 (unit: kpc)"
echo " [c]: optional; if specified, do not calculate the errors"
exit 1
fi
export PATH="/usr/local/bin:/usr/bin:/bin:$PATH"
mass_cfg="$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
abund=`grep '^abund' ${mass_cfg} | awk '{ print $2 }'`
tprofile_data=`grep '^tprofile_data' ${mass_cfg} | awk '{ print $2 }'`
tprofile_cfg=`grep '^tprofile_cfg' ${mass_cfg} | awk '{ print $2 }'`
sbp_cfg=`grep '^sbp_cfg' ${mass_cfg} | awk '{ print $2 }'`
sbp_data=`grep '^sbp_data' ${sbp_cfg} | awk '{ print $2 }'`
tprofile=`grep '^tprofile' ${sbp_cfg} | awk '{ print $2 }'`
z=`grep '^z' ${sbp_cfg} | awk '{ print $2 }'`
cm_per_pixel=`grep '^cm_per_pixel' ${sbp_cfg} | awk '{ print $2 }'`
if grep -q '^beta2' $sbp_cfg; then
MODEL="dbeta"
else
MODEL="beta"
fi
PROG_TPROFILE="fit_wang2012_model"
tprofile_dump="wang2012_dump.qdp"
${base_path}/${PROG_TPROFILE} ${tprofile_data} ${tprofile_cfg} \
${cm_per_pixel} 2> /dev/null
mv -fv ${tprofile_dump} ${tprofile}
# energy bands for which the cooling function data will be calculated
BLIST="blist.txt"
[ -e "${BLIST}" ] && mv -f ${BLIST} ${BLIST}_bak
cat > ${BLIST} << _EOF_
bolo
0.7 7
0.1 2.4
_EOF_
# NOTE:
# Set 'nh=0' when calculating the cooling function values, and use the
# value given by 'flux' with unit 'erg/s/cm^2'.
${base_path}/calc_coolfunc_bands.sh ${tprofile} ${abund} \
0 ${z} "cfunc_" ${BLIST}
PROG="calc_lx_${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_profile.py ${tprofile_data} tmp_tprofile.txt
${base_path}/shuffle_profile.py ${sbp_data} tmp_sbprofile.txt
# temperature profile
${base_path}/${PROG_TPROFILE} tmp_tprofile.txt ${tprofile_cfg} \
${cm_per_pixel} 2> /dev/null
mv -f ${tprofile_dump} ${tprofile}
TMP_SBP_CFG="tmp_sbp.cfg"
[ -e "${TMP_SBP_CFG}" ] && rm -f ${TMP_SBP_CFG}
cat ${sbp_cfg} | while read l; do
if echo "${l}" | grep -q '^sbp_data' >/dev/null; then
echo "sbp_data tmp_sbprofile.txt" >> ${TMP_SBP_CFG}
elif echo "${l}" | grep -q '^tprofile' >/dev/null; then
echo "tprofile ${tprofile}" >> ${TMP_SBP_CFG}
else
echo "${l}" >> ${TMP_SBP_CFG}
fi
done
echo "### `pwd -P`"
echo "### ${i} / ${MC_TIMES} ###"
${base_path}/calc_coolfunc_bands.sh ${tprofile} ${abund} \
0 ${z} "cfunc_" ${BLIST}
${base_path}/${PROG} ${TMP_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}
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