#!/bin/sh # # extract background spectra from src and blanksky # renormalization the blank spectrum # # References: # * Chandra spectrum analysis # http://cxc.harvard.edu/ciao/threads/extended/ # * specextract # http://cxc.harvard.edu/ciao/ahelp/specextract.html # * CIAO v4.4 region bugs # http://cxc.harvard.edu/ciao/bugs/regions.html#bug-12187 # # Weitian LI # 2012-07-24 # Change logs: # 2017-02-26, Weitian LI # * Use 'manifest.py', 'results.py', and 'renorm_spectrum.py' # * Simplify 'specextract' parameters handling # v5.0, 2015/06/02, Weitian LI # * Removed 'GREP_OPTIONS' and replace 'grep' with '\grep' # * Removed 'trap INT date' # * Copy needed pfiles to current working directory, and # set environment variable $PFILES to use these first. # * replaced 'grppha' with 'dmgroup' to group spectra # (dmgroup will add history to fits file, while grppha NOT) # v4.1, 2014/07/29, Weitian LI # fix 'pbkfile' parameters for CIAO-4.6 # 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 # v3, 2012/08/09 # fix `scientific notation' for `bc' # change `spec group' method to `min 15' # ## usage, help {{{ case "$1" in -[hH]*|--[hH]*) printf "usage:\n" printf " `basename $0` reg= [ evt= blank= nh= z= grouptype= grouptypeval= binspec= log= ]\n" printf "\nNotes:\n" printf " If grouptype=NUM_CTS, then grouptypeval required.\n" printf " If grouptype=BIN, then binspec required.\n" exit ${ERR_USG} ;; esac ## usage, help }}} ## default parameters {{{ # default `event file' which used to match `blanksky' files DFT_EVT=$(manifest.py -b getpath -r evt2_clean) # default `blanksky file' DFT_BLANK=$(manifest.py -b getpath -r bkg_blank) # default parameters for 'dmgroup' DFT_GROUPTYPE="NUM_CTS" DFT_GROUPTYPEVAL="20" #DFT_GROUPTYPE="BIN" DFT_BINSPEC="1:128:2,129:256:4,257:512:8,513:1024:16" # default `log file' DFT_LOGFILE="bkg_spectra_`date '+%Y%m%d'`.log" ASOL=$(manifest.py -b -s "," getpath -r asol) BPIX=$(manifest.py -b getpath -r bpix) MSK=$(manifest.py -b getpath -r msk) ## 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 ${keyval} shift # shift, process next one done } ## functions end }}} ## parameters {{{ # process cmdline args using `getopt_keyval' getopt_keyval "$@" ## 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 N_H=$(results.py -b get nh) else N_H=${nh} fi printf "## use nH: ${N_H}\n" | ${TOLOG} # check given redshift if [ -z "${z}" ]; then REDSHIFT=$(results.py -b get z) else REDSHIFT=${z} fi printf "## use redshift: ${REDSHIFT}\n" | ${TOLOG} # check given dmgroup parameters: grouptype, grouptypeval, binspec if [ -z "${grouptype}" ]; then GROUPTYPE="${DFT_GROUPTYPE}" elif [ "x${grouptype}" = "xNUM_CTS" ] || [ "x${grouptype}" = "xBIN" ]; then GROUPTYPE="${grouptype}" else printf "ERROR: given grouptype \`${grouptype}' invalid.\n" exit ${ERR_GRPTYPE} fi printf "## use grouptype: \`${GROUPTYPE}'\n" | ${TOLOG} if [ ! -z "${grouptypeval}" ]; then GROUPTYPEVAL="${grouptypeval}" else GROUPTYPEVAL="${DFT_GROUPTYPEVAL}" fi printf "## use grouptypeval: \`${GROUPTYPEVAL}'\n" | ${TOLOG} if [ ! -z "${binspec}" ]; then BINSPEC="${binspec}" else BINSPEC="${DFT_BINSPEC}" fi printf "## use binspec: \`${BINSPEC}'\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 }}} ## prepare parameter files (pfiles) {{{ CIAO_TOOLS="dmstat dmkeypar dmhedit specextract dmextract dmgroup" # Copy necessary pfiles for localized usage for tool in ${CIAO_TOOLS}; do pfile=`paccess ${tool}` [ -n "${pfile}" ] && punlearn ${tool} && cp -Lvf ${pfile} . done # Modify environment variable 'PFILES' to use local pfiles first export PFILES="./:${PFILES}" ## pfiles }}} ## 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" printf "use \`specextract' to generate spectra and response ...\n" ## 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 `dmgroup') punlearn specextract specextract infile="${EVT}[sky=region(${REG_TMP})]" \ outroot=${LBKG_PI%.pi} bkgfile="" asp="${ASOL}" \ mskfile="${MSK}" badpixfile="${BPIX}" \ correctpsf=no weight=yes weight_rmf=yes \ energy="0.3:11.0:0.01" channel="1:1024:1" \ bkgresp=no combine=no binarfwmap=2 \ grouptype=NONE binspec=NONE \ clobber=yes verbose=2 # 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" renorm_spectrum.py -r ${LBKG_PI} ${BBKG_PI} ## bkg renorm }}} ## group spectrum {{{ # use 'dmgroup' instead of 'grppha', because 'dmgroup' will add # command history to FITS header (maybe useful for later reference). printf "group spectrum using \`dmgroup'\n" LBKG_GRP_PI="${LBKG_PI%.pi}_grp.pi" punlearn dmgroup dmgroup infile="${LBKG_PI}" outfile="${LBKG_GRP_PI}" \ grouptype="${GROUPTYPE}" grouptypeval=${GROUPTYPEVAL} \ binspec="${BINSPEC}" xcolumn="CHANNEL" ycolumn="COUNTS" \ clobber=yes ## group }}} ## generate a script for XSPEC {{{ XSPEC_XCM="xspec_${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: #