Download Analysis Cookbook - CASA
Transcript
APPENDIX A. APPENDIX: SINGLE DISH DATA PROCESSING 307 specunit -- units for spectral axis options: (str) ’channel’,’km/s’,’GHz’,’MHz’,’kHz’,’Hz’ default: ’’ (=current) example: this will be the units for masklist frame -- frequency frame for spectral axis options: (str) ’LSRK’,’REST’,’TOPO’,’LSRD’,’BARY’, ’GEO’,’GALACTO’,’LGROUP’,’CMB’ default: currently set frame in scantable WARNING: frame=’REST’ not yet implemented doppler -- doppler mode options: (str) ’RADIO’,’OPTICAL’,’Z’,’BETA’,’GAMMA’ default: currently set doppler in scantable scanaverage -- average integrations within scans options: (bool) True,False default: False example: if True, this happens in read-in For GBT, set False! timeaverage -- average times for multiple scan cycles options: (bool) True,False default: False example: if True, this happens after calibration polaverage -- average polarizations options: (bool) True,False default: False outfile -- Name of output file default: ’’ (scantable) example: outform -- format of output file options: ’ASCII’,’SDFITS’,’MS’,’ASAP’ default: ’ASAP’ example: the ASAP format is easiest for further sd processing; use MS for CASA imaging. If ASCII, then will append some stuff to the outfile name overwrite -- overwrite the output file if already exists options: (bool) True,False default: False WARNING: if outform=’ASCII’, this parameter is ignored DESCRIPTION: Task sdcoadd merges multiple single dish spectral data given by a list of spectral data file names in any of the following formats, ASAP, MS2, and SDFITS. The units of line flux, the units of spectral axis, frame, and doppler are assumed to be those of the first one in the sdfilelist if not specified. The timaverage and polaverage are used to perform time and polarization averaging over scans on the merged scantable to obtained co-added spectra before saving to a file on disk.
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