Fig. 6

Final VLA-COSMOS 3 GHz MSMF mosaic with overlaid Gaussian fits to the pixel surface brightness distributions in various mosaic sectors. The rms obtained via the Gaussian fit (in units of μJy beam-1) is indicated in each panel. The panels shown cover the full COSMOS two square degree field. The small-scale (~1′) rms variations due to the pointing layout are less than 2%.
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