Planck 2013 results
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Fig. 2


Blind S/N versus S/N re-extracted at the X-ray position using the X-ray size, for the MMF3 detections of Planck clusters that are associated with known X-ray clusters in the reference cosmological sample. In contrast to the blind SZ flux, the blind S/N is in good agreement with S/N measured using X-ray priors.

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