Planck 2015 results
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Fig. 16


Comparison between the Metsähovi and the colour-corrected PCCS2 flux densities (DETFLUX) interpolated to 37 GHz using 30 and 44 GHz (top) and 30 and 70 GHz (bottom). The multiple observations of each source have been averaged to a single flux density; the averaging was performed over the period of the full Planck mission, not just the epochs at which each source was observed by Planck. The uncertainties, therefore, reflect the variability of the sources instead of the flux-density accuracy of the measurements, which is of the order of a few mJy.

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