If you decide to retain the spectral information, whether you are interested in continuum or spectral line data, then the editing procedure is more time consuming. This is obviously because of the additional dimension and no-one wants to fossick through every channel, one by one. There are two approaches to editing the spectral data base.
See the discussion on TVFLG in § 7.1 for some help on how to use SPFLG.
SPFLG | |
docat=1 | Catalogue master work file |
in2seq=0 | Create new master work file or |
in2seq=2 | Select old master work file |
with sequence number 2 | |
sources=' ' | Select all sources |
timerang=0 | Select all times |
stokes='I' | Display Stokes I or Stokes |
stokes='RR' | RR or LL if polarization |
stokes='LL' | trickery (really XX,YY) invoked |
freqid=1 | Select desired frequency |
bchan=1 | Select all channels |
echan=0 | |
antennas=0 | Select all baselines for |
baseline=0 | sequential display |
docalib=-1 | No calibration |
flagver=0 | Write to highest version of FG table |
already present or make a new one | |
doband=-1 | No bandpass to apply |
dparm=0 | |
dparm(6)=10 | Set minimum integration time in seconds |
Last update : 03/03/94
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