#!/bin/csh -f #handling daul receivers non-polarization hybrid-resolution data # #Responsible: Jun-Hui Zhao (SAO) #Version 1.1 #jhz 2011-02-25 created for reduction of the USB data which # contains the CO line in 340 receiver. #jhz 2011-03-05 separated antenna-based tsys for different receivers. #jhz 2011-03-10 tested the new methods for handling tsys. #jhz 2011-03-17 added CO identification with the JPL catalog. #jhz 2011-03-25 added LSB data from both receivers for continuum. #jhz 2011-04-01 using different color palette for illustration figure #jhz 2011-04-25 updated the figures #jhz 2011-05-06 updated the instruction lines #jhz 2011-05-18 added goto tags, and tested smauvspec # correct typo in deleting file name # # testing data: 101007_06:42:16 from Ken (Taco) Young, PI: Charlie Qi # The data set has not been moved to the public domain yet. # Please get the PI's permission for use of the testing data # and the figures produced from this script. # # demo illustration figures # fig1.ps = continuum image of dmtau # fig2.ps = spectrum from the vis data of dmtau # fig3.ps = spectrum from CO(3-2) line image cube dmtau # fig4.ps = image of integrated CO(3-2) line flux dmtau # set darea=/sma/SMAusers/jzhao/data/101007_06:42:16 set outf=101007 #goto continue # ######################################### # enable one of the next several goto # lines allow users to restart the script # from a working step. ######################################### # # #goto SMALOD #Load smadata goto INSPECT #Inspect visdata #goto TSYSFIX #Corrections for fringe amplitude #goto BPCAL #Bandpass calibration #goto APPLYBP #Apply bandpass solutions #goto GCAL #Gain calibration for target #goto FLUX #Determine flux density scale #goto SPLIT #Split the data into single-source file #goto LCSEPARATE #Line and continuum separation #goto CONTMAP #make continuum map #goto LIDENTIFY #molecular line identification #goto LINECUBE #make line image cube #goto MOMENTMAP #make moment map #goto DIAPLAY #display the result # SMALOD: ############################################## echo "1. READ THE MIR DATA INTO MIRIAD" ############################################## \rm -r ${outf}_rxl.* smalod in=$darea out=$outf \ rxif=-1 sideband=2 \rm -r ${outf}_rxh.* smalod in=$darea out=$outf \ rxif=-2 sideband=2 $< INSPECT: ############################################## echo "2. INSPECT THE DATA" ############################################## uvindex vis=${outf}_rxl.usb $< uvindex vis=${outf}_rxh.usb $< uvindex vis=${outf}_rxl.lsb $< uvindex vis=${outf}_rxh.lsb $< smauvplt vis=${outf}_rxl.usb \ axis=time,ampl device=/xs nxy=1,1 $< smauvplt vis=${outf}_rxh.usb \ axis=time,ampl device=/xs nxy=1,1 $< smauvplt vis=${outf}_rxl.lsb \ axis=time,ampl device=/xs nxy=1,1 $< smauvplt vis=${outf}_rxh.lsb \ axis=time,ampl device=/xs nxy=1,1 $< smauvspec vis=${outf}_rxl.usb \ select='source(dmtau)' \ interval=1000 hann=1 \ axis=chan,both device=/xs nxy=1,3 $< smauvspec vis=${outf}_rxh.usb \ select='source(dmtau)' \ interval=1000 hann=1 \ axis=chan,both device=/xs nxy=1,3 smauvspec vis=${outf}_rxl.lsb \ select='source(dmtau)' \ interval=1000 hann=1 \ axis=chan,both device=/xs nxy=1,3 $< smauvspec vis=${outf}_rxh.lsb \ select='source(dmtau)' \ interval=1000 hann=1 \ axis=chan,both device=/xs nxy=1,3 $< smavarplt vis=${outf}_rxl.usb device=/xs \ xaxis=time \ yaxis=systemp nxy=2,4 $< smavarplt vis=${outf}_rxh.usb device=/xs \ xaxis=time \ yaxis=systemp nxy=2,4 $< smavarplt vis=${outf}_rxl.lsb device=/xs \ xaxis=time \ yaxis=systemp nxy=2,4 $< smavarplt vis=${outf}_rxh.lsb device=/xs \ xaxis=time \ yaxis=systemp nxy=2,4 $< TSYSFIX: ################################################### echo "3. CORRECTIONS FOR FRINGE AMPLITUDE" ################################################### $< \rm -r ${outf}_rxl.usb.tsys smafix vis=${outf}_rxl.usb out=${outf}_rxl.usb.tsys \ device=/xs xaxis=time \ yaxis=systemp nxy=2,4 \ options=tsyscorr $< \rm -r ${outf}_rxh.usb.tsys smafix vis=${outf}_rxh.usb out=${outf}_rxh.usb.tsys \ device=/xs xaxis=time \ yaxis=systemp nxy=2,4 \ options=tsyscorr $< \rm -r ${outf}_rxl.lsb.tsys smafix vis=${outf}_rxl.lsb out=${outf}_rxl.lsb.tsys \ device=/xs xaxis=time \ yaxis=systemp nxy=2,4 \ options=tsyscorr $< \rm -r ${outf}_rxh.lsb.tsys smafix vis=${outf}_rxh.lsb out=${outf}_rxh.lsb.tsys \ device=/xs xaxis=time \ yaxis=systemp nxy=2,4 \ options=tsyscorr $< smablflag vis=${outf}_rxl.usb.tsys \ axis=time,ampl device=/xs $< smablflag vis=${outf}_rxh.usb.tsys \ axis=time,ampl device=/xs $< smablflag vis=${outf}_rxl.lsb.tsys \ axis=time,ampl device=/xs $< smablflag vis=${outf}_rxh.lsb.tsys \ axis=time,ampl device=/xs $< smauvspec vis=${outf}_rxl.usb.tsys \ select='source(3c454.3)' \ interval=1000 \ axis=freq,both device=/xs nxy=1,5 $< smauvspec vis=${outf}_rxh.usb.tsys \ select='source(3c454.3)' \ interval=1000 \ axis=freq,both device=/xs nxy=1,5 $< smauvspec vis=${outf}_rxl.lsb.tsys \ select='source(3c454.3)' \ interval=1000 \ axis=freq,both device=/xs nxy=1,5 $< smauvspec vis=${outf}_rxh.lsb.tsys \ select='source(3c454.3)' \ interval=1000 \ axis=freq,both device=/xs nxy=1,5 $< BPCAL: ######################################### echo '4. BANDPASS CALIBRATION' ######################################### smamfcal vis=${outf}_rxl.usb.tsys select='source(3c454.3)' edge=8,8 \ weight=2 refant=3 interval=60000 $< smagpplt vis=${outf}_rxl.usb.tsys device=/xs \ yaxis=amp,phase \ options=bandpass polyfit=5 \ nxy=1,8 smamfcal vis=${outf}_rxh.usb.tsys select='source(3c454.3)' edge=8,8 \ weight=2 refant=3 interval=60000 $< smagpplt vis=${outf}_rxh.usb.tsys device=/xs \ yaxis=amp,phase \ options=bandpass polyfit=5 \ nxy=1,8 smamfcal vis=${outf}_rxl.lsb.tsys select='source(3c454.3)' edge=8,8 \ weight=2 refant=3 interval=60000 $< smagpplt vis=${outf}_rxl.lsb.tsys device=/xs \ yaxis=amp,phase \ options=bandpass polyfit=5 \ nxy=1,8 smamfcal vis=${outf}_rxh.lsb.tsys select='source(3c454.3)' edge=8,8 \ weight=2 refant=3 interval=60000 $< smagpplt vis=${outf}_rxh.lsb.tsys device=/xs \ yaxis=amp,phase \ options=bandpass polyfit=5 \ nxy=1,8 $< APPLYBP: ##################################### # Apply bandpass calibration ##################################### # \rm -r ${outf}_rxl.usb.tsys.bp ${outf}_rxh.usb.tsys.bp uvaver vis=${outf}_rxl.usb.tsys options=nocal \ out=${outf}_rxl.usb.tsys.bp $< uvaver vis=${outf}_rxh.usb.tsys options=nocal \ out=${outf}_rxh.usb.tsys.bp \rm -r ${outf}_rxl.lsb.tsys.bp ${outf}_rxh.lsb.tsys.bp uvaver vis=${outf}_rxl.lsb.tsys options=nocal \ out=${outf}_rxl.lsb.tsys.bp $< uvaver vis=${outf}_rxh.lsb.tsys options=nocal \ out=${outf}_rxh.lsb.tsys.bp $< GCAL: ################################################# echo '5. GAIN CALIBRATION' ################################################# $< smamfcal vis=${outf}_rxl.usb.tsys.bp \ select='source(0449+113)' \ refant=3 interval=2 options=nopassol $< smagpplt vis=${outf}_rxl.usb.tsys.bp device=/xs \ yaxis=amp,pha \ options=gains polyfit=6 \ nxy=2,4 smamfcal vis=${outf}_rxh.usb.tsys.bp \ select='source(0449+113)' \ refant=3 interval=2 options=nopassol $< smagpplt vis=${outf}_rxh.usb.tsys.bp device=/xs \ yaxis=amp,pha \ options=gains polyfit=6 \ nxy=2,4 $< smamfcal vis=${outf}_rxl.lsb.tsys.bp \ select='source(0449+113)' \ refant=3 interval=2 options=nopassol $< smagpplt vis=${outf}_rxl.lsb.tsys.bp device=/xs \ yaxis=amp,pha \ options=gains polyfit=6 \ nxy=2,4 smamfcal vis=${outf}_rxh.lsb.tsys.bp \ select='source(0449+113)' \ refant=3 interval=2 options=nopassol $< smagpplt vis=${outf}_rxh.lsb.tsys.bp device=/xs \ yaxis=amp,pha \ options=gains polyfit=6 \ nxy=2,4 \rm -r ${outf}_rxl.usb.tsys.bp.g ${outf}_rxh.usb.tsys.bp.g uvaver vis=${outf}_rxl.usb.tsys.bp \ out=${outf}_rxl.usb.tsys.bp.g $< uvaver vis=${outf}_rxh.usb.tsys.bp \ out=${outf}_rxh.usb.tsys.bp.g \rm -r ${outf}_rxl.lsb.tsys.bp.g ${outf}_rxh.lsb.tsys.bp.g uvaver vis=${outf}_rxl.lsb.tsys.bp \ out=${outf}_rxl.lsb.tsys.bp.g $< uvaver vis=${outf}_rxh.lsb.tsys.bp \ out=${outf}_rxh.lsb.tsys.bp.g $< FLUX: ############################################ echo '6. BOOTSTRAPE THE FLUX DENSITY SCALE' ############################################ $< smaflux vis=${outf}_rxl.usb.tsys.bp.g \ select='source(callisto)' mirhome=$MIR $< smaflux vis=${outf}_rxh.usb.tsys.bp.g \ select='source(callisto)' mirhome=$MIR $< smaflux vis=${outf}_rxl.lsb.tsys.bp.g \ select='source(callisto)' mirhome=$MIR $< smaflux vis=${outf}_rxh.lsb.tsys.bp.g \ select='source(callisto)' mirhome=$MIR $< \rm -r ${outf}_rxl.usb.tsys.bp.ga ${outf}_rxh.usb.tsys.bp.ga uvaver vis=${outf}_rxl.usb.tsys.bp.g \ out=${outf}_rxl.usb.tsys.bp.ga $< uvaver vis=${outf}_rxh.usb.tsys.bp.g \ out=${outf}_rxh.usb.tsys.bp.ga $< \rm -r ${outf}_rxl.lsb.tsys.bp.ga ${outf}_rxh.lsb.tsys.bp.ga uvaver vis=${outf}_rxl.lsb.tsys.bp.g \ out=${outf}_rxl.lsb.tsys.bp.ga $< uvaver vis=${outf}_rxh.lsb.tsys.bp.g \ out=${outf}_rxh.lsb.tsys.bp.ga SPLIT: ################################### # Split visibility on source based. ################################### $< \rm -r dmtau.345233 dmtau.371859 dmtau.usb.350 dmtau.usb.400 uvsplit vis=${outf}_rxl.usb.tsys.bp.ga select='source(dmtau)' \ options=nowindow uvsplit vis=${outf}_rxh.usb.tsys.bp.ga select='source(dmtau)' \ options=nowindow \rm -r dmtau.337111 dmtau.363737 dmtau.lsb.350 dmtau.lsb.400 uvsplit vis=${outf}_rxl.lsb.tsys.bp.ga select='source(dmtau)' \ options=nowindow uvsplit vis=${outf}_rxh.lsb.tsys.bp.ga select='source(dmtau)' \ options=nowindow $< mv dmtau.345233 dmtau.usb.350 mv dmtau.371859 dmtau.usb.400 mv dmtau.337111 dmtau.lsb.350 mv dmtau.363737 dmtau.lsb.400 $< LCSEPARATE: ################################### # Line and continuum separation ################################### $< \rm -r dmtau.usb.350.ch0 dmtau.usb.400.ch0 uvlin vis=dmtau.usb.350 chans=1,3008 out=dmtau.usb.350.ch0 \ order=1 mode=chan0 options=nowin $< uvlin vis=dmtau.usb.350 chans=1,3008 out=dmtau.usb.400.ch0 \ order=1 mode=chan0 options=nowin $< \rm -r dmtau.lsb.350.ch0 dmtau.lsb.400.ch0 uvlin vis=dmtau.lsb.350 chans=1,3008 out=dmtau.lsb.350.ch0 \ order=1 mode=chan0 options=nowin $< uvlin vis=dmtau.lsb.350 chans=1,3008 out=dmtau.lsb.400.ch0 \ order=1 mode=chan0 options=nowin CONTMAP: ############################################# echo "7. CONTINUUM IMAGE" ############################################# $< \rm -r dmtau.map dmtau.beam dmtau.icmp set visdata=dmtau.usb.400.ch0,dmtau.lsb.400.ch0,dmtau.usb.350.ch0,dmtau.lsb.350.ch0 invert vis=${visdata} map=dmtau.map beam=dmtau.beam \ imsize=512,512 cell=0.3 robust=2 \ options=systemp $< cgdisp in=dmtau.map type=pixel region=arcsec,'boxes(-15,-15,15,15)' \ xybin=1,1 device=/xs nxy=1,1 options=full,beambr,wedge \ labtyp=arcsec,arcsec range=0,0,lin,2 cols1=7 csize=1,1 $< clean map=dmtau.map beam=dmtau.beam out=dmtau.icmp gain=0.08 \ cutoff=0 niters=5000 \ region=arcsec,'boxes(-1,-1,1,1)' $< \rm -r dmtau.icln restor model=dmtau.icmp beam=dmtau.beam map=dmtau.map \ out=dmtau.icln $< cgdisp in=dmtau.icln type=pixel region=arcsec,'boxes(-15,-15,15,15)' \ xybin=1,1 device=fig1.ps/cps nxy=1,1 options=beambr,wedge,blacklab \ labtyp=arcsec,arcsec range=0.005,0.14,lin,2 cols1=7 csize=1,1 $< imstat in=dmtau.icln region=arcsec,'boxes(-15,-15,-12,-12)' \ axes=ra,dec $< \rm -r dmtau.345800 uvsplit vis=dmtau.usb.350 select='window(8)' $< mv dmtau.345800 dmtau.co $< LIDENTIFY: #################################################### echo "8. LINE IDENTIFICATION" #################################################### $< #... #skip #select 27002 HNC ( y to select it or n to skip it or t to terminate) #n #skip #select 27003 HCN-v2 ( y to select it or n to skip it or t to terminate) #n #skip #select 27004 C-13-N ( y to select it or n to skip it or t to terminate) #n #skip #select 28001 CO ( y to select it or n to skip it or t to terminate) #y #yes #select 28002 HC-13-N ( y to select it or n to skip it or t to terminate) #t #terminate selection smauvspec vis=dmtau.usb.350 hann=15 select='source(dmtau)' \ interval=1000 options=nobase,avall,jplcat,restfreq \ axis=freq,both device=fig2.ps/cps nxy=1,1 \ vsource=6.5 veltype=lsr catpath=$MIRCAT/jplcat veldef=radio $< \rm -r dmtau.co.lin uvlin vis=dmtau.co chans=1,100,170,250 out=dmtau.co.lin \ order=1 mode=line options=nowin $< smauvspec vis=dmtau.co.lin hann=7 \ interval=1000 options=avall,nobase \ axis=freq,both device=/xs nxy=1,1 $< LINECUBE: #################################################### echo '9. LINE IMAGING' #################################################### $< \rm -r dmtau.l.map dmtau.l.beam dmtau.l.icmp invert vis=dmtau.co.lin map=dmtau.l.map beam=dmtau.l.beam \ imsize=1024,1024 cell=0.2 robust=0 \ options=systemp line=vel,100,-10,0.35 $< clean map=dmtau.l.map beam=dmtau.l.beam out=dmtau.l.icmp gain=0.08 \ cutoff=0.05 niters=10000 \ region=arcsec,'boxes(-20,-20,20,20)(1,100)' $< \rm -r dmtau.l.icln restor model=dmtau.l.icmp beam=dmtau.l.beam map=dmtau.l.map \ out=dmtau.l.icln $< cgdisp in=dmtau.l.icln type=pixel \ region=arcsec,'boxes(-15,-15,15,15)(1,100)' \ xybin=1,1 device=/xs nxy=5,5 options=beambr,wedge,blacklab \ labtyp=arcsec,arcsec range=0,0,lin,2 cols1=7 csize=1,1 $< imstat in=dmtau.l.icln region=arcsec,'boxes(-25,-25,-22,-22)' \ axes=ra,dec $< MOMENTMAP: ##################################### echo "spectrum of the CO line" ##################################### $< imspect in=dmtau.l.icln region=arcsec,'boxes(-0.,-0.,0.,0.)(1,100)' \ device=fig3.ps/ps yrange=-0.5,2. $< \rm -r dmtau.l.flux moment in==dmtau.l.icln region='quarter(20,70)' out=dmtau.l.flux mom=0 \ clip=-10,0.25 $< DISPLAY: ###################################### echo "10. DISPLAY THE LINE FLUX IMAGE" ###################################### $< cgdisp in=dmtau.l.flux,dmtau.l.flux type=c,p \ region=arcsec,'boxes(-8,-8.5,8,7.5)' \ xybin=1,1 device=fig4.ps/cps nxy=1,1 options=beambr,wedge,blacklab \ labtyp=arcsec,arcsec range=0.01,4,lin,8 cols1=3 csize=1.2,1.2 \ slev=p,1 levs1=6,10,15,25,35,45,55,65,75,85,95 exit