# plotants :: Plot the antenna distribution in the local reference frame: We'd like our reference antenna to be near the center of the array, and the easiest way to envision the array layout is with plotants. There are no cross-polarization data (note that 'Corrs' is set to only 'RR LL'). This window is sampled with 256 channels each 7.8 kHz wide. The correlator is set up in such a way to have one spectral window (or IF). Some things to note here are: The phase calibrator is called J1042+1203, the flux calibrator is 1331+305, and there are two science pointings, Leo-1 and Leo-2. 18:11:35 INFO listobs # End Task: listobs # 18:11:35 INFO listobs ID Name Station Diam. 18:11:35 INFO listobs ID Name SpwId RestFreq(MHz) SysVel(km/s) 18:11:35 INFO listobs SpwID #Chans Frame Ch1(MHz) ChanWid(kHz)TotBW(kHz) Ref(MHz) Corrs 18:11:35 INFO listobs Spectral Windows: (1 unique spectral windows and 1 unique polarization setups) 18:11:35 INFO listobs (nVis = Total number of time/baseline visibilities per field) 18:11:35 INFO listobs ID Code Name RA Decl Epoch SrcId nVis 18:11:35 INFO listobs (nVis = Total number of time/baseline visibilities per scan) 18:11:35 INFO listobs Date Timerange (UTC) Scan FldId FieldName nVis Int(s) SpwIds 18:11:35 INFO listobs ObservationID = 0 ArrayID = 0 18:11:34 INFO listobsĝata records: 70290 Total integration time = 11264.5 seconds 18:11:34 INFO listobs Observer: leo2pt Project: T.B.D. 18:11:34 INFO listobs MeasurementSet Name: /export/home/rso-lchomiuk/test/Leo/leotest.ms MS Version 2 18:11:34 INFO listobs # Begin Task: listobs # Listobs will produce output that looks like this:
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