Imaging a Mosaicked Spectral Line Dataset
As before, these notes assume that you have made the following global definitions in CASA:
# In CASA msdir='./' project='c0xxx' msfile=msdir+project+'.ms'
If your data are already edited and calibrated, there's really only one step left: clean. Unlike in MIRIAD, which has separate tasks for inverting and cleaning an image, CASA does it in one step. If you want a dirty image, just set niter=0 so that clean doesn't actually do any...cleaning.
Here's a command-line call to clean, which demonstrates many of the interesting parameters you can tweak. This is a simple example, assuming you are making an image of a single field, and you want to clean the whole thing.
Some things of note:
- phasecenter doesn't need to be specified, if you are happy with the phase center that clean derives from the combined mosaicked fields.
- it is important for both imagermode and ftmachine to be set to 'mosaic' if you want your mosaicked data to be stitched together correctly.
- always include units when specifying the threshold at which to stop cleaning.
# In CASA clean(vis=msfile,imagename='clean_pb',spw='1,2',field='3~51', phasecenter='J2000 20h35m35.32 60d10m01.00', cell=2.,imsize=[400,400], mode='velocity',start='-103.00km/s',width='5.08km/s',nchan=29, interpolation='linear',psfmode='clark', imagermode='mosaic',ftmachine='mosaic', scaletype='SAULT',restfreq='115.2712GHz',interactive=F, minpb=0.1,pbcor=True, niter=1000,threshold='340mJy',mosweight=False, weighting='natural')