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The proposed VLA Sky Survey (VLASS) comprises two distinct S-band (2--4 GHz)surveys: (1) All-Sky covering the sky north of -40 deg with rms noise 69microJy/beam = 1.5 K in the 2.5 arcsec beam and (2) Deep covering 10 square degwith rms noise 1.5 microJy/beam = 0.32 K in the 0.8 arcsec beam. This reviewcompares the scientific goals and technical capabilities of the VLASS proposal(2015 Jan 15 version), using new calculations of performance metrics forsurveys made with large fractional bandwidths.

An Analysis of the VLASS Proposal