Logged on 06/30/2009 12:34:28 PM
This is a repeat of SSSC1 except we are now going to give the source a spectral shape.
Please refer to the PURR log for SSSC1 if you haven't already.
LSM format is a matter of preference, or perhaps convenience. The diagram below shows the required columns for the h m s, d m s text file format. The only difference between this and the LSM for SSSC1 is the value of -0.7 in the spectral index column, and the source name has been changed to SSSC11.
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Logged on 06/30/2009 12:48:06 PM
Repeating the steps as per SSSC1 now to intialise the MS columns, add the visibilities and image the result.
If you're eagle-eyed you will have noticed the differences in the histograms of this and the spectrally flat case presented in SSSC1.
Remember that you can also generate a datacube at the imaging stage.
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