Planck 2013 results
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Fig. 3

image

Comparison of the measurements of Y5R500. Left: the values derived from the detection methods used to build the Planck catalogue of clusters (Y5R500,PSZ), plotted against those from the all-sky reconstructed MILCA tSZ map (Y5R500,y − MAP). Right: the MILCA (Y5R500,MILCA) versus NILC (Y5R500,NILC) all-sky tSZ effect maps. The equality relationship is marked as a dashed black line. A least-squares bisector method fit to the data lead to slopes of 1.09 ± 0.02 and 1.08 ± 0.02 for the MILCA and NILC Compton parameter maps, respectively.

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