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This section describes single-field imaging/deconvolution for the continuum and spectral-line datasets as well as how to interactively define a CLEAN region.
There are almost as many ways to deconvolve an image as there are radio astronomers. The examples given in this section illustrate two relatively simple ways to create images. They have been designed to step the beginning user through the imaging process without getting bogged down with too many details. For an in depth discussion about imaging strategies and the imager arguments see the web documentation at synthesis imaging and imager.