#!/bin/sh - # trap date INT unalias -a export GREP_OPTIONS="" export LC_COLLATE=C ########################################################### ## extract background spectra from src and blanksky ## ## renormalization the blank spectrum ## ## ## ## Ref: Chandra spectrum analysis ## ## http://cxc.harvard.edu/ciao/threads/extended/ ## ## Ref: specextract ## ## http://cxc.harvard.edu/ciao/ahelp/specextract.html ## ## Ref: CIAO v4.4 region bugs ## ## http://cxc.harvard.edu/ciao/bugs/regions.html#bug-12187 ## ## ## LIweitiaNux, July 24, 2012 ## ########################################################### ########################################################### # ChangeLogs: # v3, 2012/08/09 # fix `scientific notation' for `bc' # change `spec group' method to `min 15' # v4, 2012/08/13 # add `clobber=yes' # improve error code # improve cmdline arguements # provide a flexible way to pass parameters # (through cmdline which similar to CIAO, # and default filename match patterns) # add simple `logging' function # v4.1, 2014/07/29, Weitian LI # fix 'pbkfile' parameters for CIAO-4.6 ########################################################### ## about, used in `usage' {{{ VERSION="v4" UPDATE="2012-08-14" ## about }}} ## usage, help {{{ case "$1" in -[hH]*|--[hH]*) printf "usage:\n" printf " `basename $0` evt= reg= blank= basedir= nh= z= [ grpcmd= log= ]\n" printf "\nversion:\n" printf "${VERSION}, ${UPDATE}\n" exit ${ERR_USG} ;; esac ## usage, help }}} ## default parameters {{{ # default `event file' which used to match `blanksky' files #DFT_EVT="_NOT_EXIST_" DFT_EVT="`ls evt2*_clean.fits`" # default `blanksky file' #DFT_BLANK="_NOT_EXIST_" DFT_BLANK="`ls blanksky*.fits`" # default dir which contains `asols, asol.lis, ...' files #DFT_BASEDIR="_NOT_EXIST_" DFT_BASEDIR=".." # default `group command' for `grppha' #DFT_GRP_CMD="group 1 128 2 129 256 4 257 512 8 513 1024 16" DFT_GRP_CMD="group min 20" # default `log file' DFT_LOGFILE="bkg_spectra_`date '+%Y%m%d'`.log" ## howto find files in `basedir' # default `asol.lis pattern' DFT_ASOLIS_PAT="acis*asol?.lis" # default `bad pixel filename pattern' DFT_BPIX_PAT="acis*repro*bpix?.fits" # default `pbk file pattern' DFT_PBK_PAT="acis*pbk?.fits" # default `msk file pattern' DFT_MSK_PAT="acis*msk?.fits" ## default parameters }}} ## error code {{{ ERR_USG=1 ERR_DIR=11 ERR_EVT=12 ERR_BKG=13 ERR_REG=14 ERR_ASOL=21 ERR_BPIX=22 ERR_PBK=23 ERR_MSK=24 ERR_BKGTY=31 ERR_SPEC=32 ## error code }}} ## functions {{{ # process commandline arguments # cmdline arg format: `KEY=VALUE' getopt_keyval() { until [ -z "$1" ] do key=${1%%=*} # extract key val=${1#*=} # extract value keyval="${key}=\"${val}\"" echo "## getopt: eval '${keyval}'" eval ${keyval} shift # shift, process next one done } ## background renormalization (BACKSCAL) {{{ # renorm background according to particle background # energy range: 9.5-12.0 keV (channel: 651-822) CH_LOW=651 CH_HI=822 pb_flux() { punlearn dmstat COUNTS=`dmstat "$1[channel=${CH_LOW}:${CH_HI}][cols COUNTS]" | grep -i 'sum:' | awk '{ print $2 }'` punlearn dmkeypar EXPTIME=`dmkeypar $1 EXPOSURE echo=yes` BACK=`dmkeypar $1 BACKSCAL echo=yes` # fix `scientific notation' bug for `bc' EXPTIME_B=`echo ${EXPTIME} | sed 's/[eE]/\*10\^/' | sed 's/+//'` BACK_B=`echo "( ${BACK} )" | sed 's/[eE]/\*10\^/' | sed 's/+//'` PB_FLUX=`echo "scale = 16; ${COUNTS} / ${EXPTIME_B} / ${BACK_B}" | bc -l` echo ${PB_FLUX} } bkg_renorm() { # $1: src spectrum, $2: back spectrum PBFLUX_SRC=`pb_flux $1` PBFLUX_BKG=`pb_flux $2` BACK_OLD=`dmkeypar $2 BACKSCAL echo=yes` BACK_OLD_B=`echo "( ${BACK_OLD} )" | sed 's/[eE]/\*10\^/' | sed 's/+//'` BACK_NEW=`echo "scale = 16; ${BACK_OLD_B} * ${PBFLUX_BKG} / ${PBFLUX_SRC}" | bc -l` printf "\`$2': BACKSCAL:\n" printf " ${BACK_OLD} --> ${BACK_NEW}\n" punlearn dmhedit dmhedit infile=$2 filelist=none operation=add \ key=BACKSCAL value=${BACK_NEW} comment="old value: ${BACK_OLD}" } ## bkg renorm }}} ## functions end }}} ## parameters {{{ # process cmdline args using `getopt_keyval' getopt_keyval "$@" ## check log parameters {{{ if [ ! -z "${log}" ]; then LOGFILE="${log}" else LOGFILE=${DFT_LOGFILE} fi printf "## use logfile: \`${LOGFILE}'\n" [ -e "${LOGFILE}" ] && mv -fv ${LOGFILE} ${LOGFILE}_bak TOLOG="tee -a ${LOGFILE}" echo "process script: `basename $0`" >> ${LOGFILE} echo "process date: `date`" >> ${LOGFILE} ## log }}} # check given parameters # check evt file if [ -r "${evt}" ]; then EVT=${evt} elif [ -r "${DFT_EVT}" ]; then EVT=${DFT_EVT} else read -p "clean evt2 file: " EVT if [ ! -r "${EVT}" ]; then printf "ERROR: cannot access given \`${EVT}' evt file\n" exit ${ERR_EVT} fi fi printf "## use evt file: \`${EVT}'\n" | ${TOLOG} # check given region file(s) if [ -z "${reg}" ]; then read -p "> selected local bkg region file: " REGLIST else REGLIST="${reg}" fi REGLIST=`echo ${REGLIST} | tr ',' ' '` # use *space* to separate printf "## use reg file(s): \`${REGLIST}'\n" | ${TOLOG} # check given blanksky if [ -r "${blank}" ]; then BLANK=${blank} elif [ -r "${DFT_BLANK}" ]; then BLANK=${DFT_BLANK} else read -p "> matched blanksky evtfile: " BLANK if [ ! -r "${BLANK}" ]; then printf "ERROR: cannot acces given \`${BLANK}' blanksky file\n" exit ${ERR_BKG} fi fi # check given nH if [ -z "${nh}" ]; then read -p "> value of nH: " N_H else N_H=${nh} fi printf "## use nH: ${N_H}\n" | ${TOLOG} # check given redshift if [ -z "${z}" ]; then read -p "> value of redshift: " REDSHIFT else REDSHIFT=${z} fi printf "## use redshift: ${REDSHIFT}\n" | ${TOLOG} # check given dir if [ -d "${basedir}" ]; then BASEDIR=${basedir} elif [ -d "${DFT_BASEDIR}" ]; then BASEDIR=${DFT_BASEDIR} else read -p "> basedir (contains asol files): " BASEDIR if [ ! -d "${BASEDIR}" ]; then printf "ERROR: given \`${BASEDIR}' NOT a directory\n" exit ${ERR_DIR} fi fi # remove the trailing '/' BASEDIR=`echo ${BASEDIR} | sed 's/\/*$//'` printf "## use basedir: \`${BASEDIR}'\n" | ${TOLOG} # check given `grpcmd' if [ ! -z "${grpcmd}" ]; then GRP_CMD="${grpcmd}" else GRP_CMD="${DFT_GRP_CMD}" fi printf "## use grppha cmd: \`${GRP_CMD}'\n" | ${TOLOG} ## parameters }}} ## check needed files {{{ # check reg file(s) printf "check accessibility of reg file(s) ...\n" for reg_f in ${REGLIST}; do if [ ! -r "${reg_f}" ]; then printf "ERROR: file \`${reg_f}' NOT accessiable\n" exit ${ERR_REG} fi done # check the validity of *pie* regions printf "check pie reg validity ...\n" INVALID=`cat ${REGLIST} | grep -i 'pie' | awk -F, '{ print $6 }' | tr -d ')' | awk '$1 > 360'` if [ "x${INVALID}" != "x" ]; then printf "WARNING: some pie region's END_ANGLE > 360\n" | ${TOLOG} printf " CIAO v4.4 tools may run into trouble\n" fi # check files in `basedir' printf "check needed files in basedir \`${BASEDIR}' ...\n" # check asolis files ASOLIS=`ls -1 ${BASEDIR}/${DFT_ASOLIS_PAT} | head -n 1` if [ -z "${ASOLIS}" ]; then printf "ERROR: cannot find \"${DFT_ASOLIS_PAT}\" in dir \`${BASEDIR}'\n" exit ${ERR_ASOL} fi printf "## use asolis: \`${ASOLIS}'\n" | ${TOLOG} # check badpixel file BPIX=`ls -1 ${BASEDIR}/${DFT_BPIX_PAT} | head -n 1` if [ -z "${BPIX}" ]; then printf "ERROR: cannot find \"${DFT_BPIX_PAT}\" in dir \`${BASEDIR}'\n" exit ${ERR_BPIX} fi printf "## use badpixel: \`${BPIX}'\n" | ${TOLOG} # check pbk file PBK=`ls -1 ${BASEDIR}/${DFT_PBK_PAT} | head -n 1` if [ -z "${PBK}" ]; then printf "ERROR: cannot find \"${DFT_PBK_PAT}\" in dir \`${BASEDIR}'\n" exit ${ERR_PBK} fi printf "## use pbk: \`${PBK}'\n" | ${TOLOG} # check msk file MSK=`ls -1 ${BASEDIR}/${DFT_MSK_PAT} | head -n 1` if [ -z "${MSK}" ]; then printf "ERROR: cannot find \"${DFT_MSK_PAT}\" in dir \`${BASEDIR}'\n" exit ${ERR_MSK} fi printf "## use msk: \`${MSK}'\n" | ${TOLOG} ## check files }}} ## main part {{{ ## use 'for' loop to process every region file for reg_i in ${REGLIST}; do printf "\n==============================\n" printf "PROCESS REGION fle \`${reg_i}' ...\n" REG_TMP="_tmp.reg" [ -f "${REG_TMP}" ] && rm -fv ${REG_TMP} # remove tmp files cp -fv ${reg_i} ${REG_TMP} # check the validity of *pie* regions {{{ INVALID=`grep -i 'pie' ${REG_TMP} | awk -F, '{ print $6 }' | tr -d ')' | awk '$1 > 360'` if [ "x${INVALID}" != "x" ]; then printf "WARNING: fix for *pie* region in file \`${reg_i}'\n" cat ${REG_TMP} A_OLD=`echo ${INVALID} | sed 's/\./\\\./'` A_NEW=`echo ${INVALID}-360 | bc -l | sed 's/\./\\\./'` sed -i'' "s/${A_OLD}\ *)/${A_NEW})/" ${REG_TMP} printf " --> " cat ${REG_TMP} fi ## check pie region }}} LBKG_PI="${reg_i%.reg}.pi" ## use `specextract' to extract local bkg spectrum {{{ # NOTE: set `binarfwmap=2' to save the time for generating `ARF' # I have tested that this bin factor has little impact on the results. # NO background response files # NO background spectrum (generate by self) # NO spectrum grouping (group by self using `grppha') # 'pbkfile' parameter deprecated in CIAO-4.6 if `pget specextract pbkfile >/dev/null 2>&1`; then P_PBKFILE="pbkfile='${PBK}'" else P_PBKFILE="" fi # printf "use \`specextract' to generate spectra and response ...\n" punlearn specextract specextract infile="${EVT}[sky=region(${REG_TMP})]" \ outroot=${LBKG_PI%.pi} bkgfile="" asp="@${ASOLIS}" \ ${P_PBKFILE} mskfile="${MSK}" badpixfile="${BPIX}" \ weight=yes correct=no bkgresp=no \ energy="0.3:11.0:0.01" channel="1:1024:1" \ combine=no binarfwmap=2 \ grouptype=NONE binspec=NONE \ verbose=2 clobber=yes # `specextract' }}} ## generate the blanksky bkg spectrum {{{ printf "generate the blanksky bkg spectrum ...\n" BBKG_PI="blanksky_${LBKG_PI}" punlearn dmextract dmextract infile="${BLANK}[sky=region(${REG_TMP})][bin pi]" \ outfile=${BBKG_PI} wmap="[bin det=8]" clobber=yes ## blanksky bkg spectrum }}} ## bkg renormalization {{{ printf "Renormalize background ...\n" bkg_renorm ${LBKG_PI} ${BBKG_PI} ## bkg renorm }}} ## group spectrum {{{ printf "group spectrum using \`grppha'\n" LBKG_GRP_PI="${LBKG_PI%.pi}_grp.pi" grppha infile="${LBKG_PI}" outfile="${LBKG_GRP_PI}" \ comm="${GRP_CMD} & exit" clobber=yes > /dev/null ## group spectra }}} ## generate a script for XSPEC {{{ XSPEC_XCM="xspec_${LBKG_PI%.pi}_model.xcm" if [ -e ${XSPEC_XCM} ]; then mv -fv ${XSPEC_XCM} ${XSPEC_XCM}_bak fi cat >> ${XSPEC_XCM} << _EOF_ ## xspec script ## analysis chandra acis background components ## xspec model: apec+apec+wabs*(pow+apec) ## ## generated by script \``basename $0`' ## `date` ## NOTES: needs XSPEC v12.x # settings statistic chi #weight churazov abund grsa query yes # data data ${LBKG_GRP_PI} response ${LBKG_PI%.pi}.wrmf arf ${LBKG_PI%.pi}.warf backgrnd ${BBKG_PI} # fitting range ignore bad ignore 0.0-0.4,8.0-** # plot related setplot energy method leven 10 0.01 xsect bcmc cosmo 70 0 0.73 xset delta 0.01 systematic 0 # model model apec + apec + wabs(powerlaw + apec) 0.08 -0.01 0.008 0.008 64 64 1 -0.001 0 0 5 5 0 -0.01 -0.999 -0.999 10 10 0.0 0.01 -1 0 0 1 0.2 -0.01 0.008 0.008 64 64 1 -0.001 0 0 5 5 0 -0.01 -0.999 -0.999 10 10 0.0 0.01 -1 0 0 1 ${N_H} -0.001 0 0 100000 1e+06 1.4 -0.01 -3 -2 9 10 0.0 0.01 -1 0 0 1 1.0 0.01 0.008 0.008 64 64 0.4 0.001 0 0 5 5 ${REDSHIFT} -0.01 -0.999 -0.999 10 10 0.0 0.01 0 0 1e+24 1e+24 freeze 1 2 3 freeze 5 6 7 freeze 9 10 14 thaw 12 13 _EOF_ ## XSPEC script }}} done # end 'for', `specextract' ## main part }}} # clean printf "clean ...\n" rm -f ${REG_TMP} printf "DONE\n" ########################################################### # vim: set ts=8 sw=4 tw=0 fenc=utf-8 ft=sh: #