The CGPS archive is very simple. The survey of the galactic plane has been segmented in different regions (or mosaics). For each mosaics, a number
of observations in multiple wavelengths / frequencies has been regridded to the same pixel scale in order to ease the comparaison.
One could find the observation nd processing status of each mosaic here
There is only a single form to query the CGPS archive using three (3) distincts methods: