Planck 2013 results
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Fig. 9

image

Comparison between the PACO sample (Massardi et al. 2011; Bonavera et al. 2011; Bonaldi et al. 2013) and the extrapolated, colour-corrected PCCS flux densities (DETFLUX) at 32 (left) and 40 GHz (right). The multiple PACO observations of each source have been averaged to a single flux density and therefore the uncertainties reflect the variability of the sources instead of the actual flux density accuracy of the measurements (a few mJy).

This figure is made of several images, please see below:

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