Compact Source Detection in Multichannel Microwave Surveys: From SZ Clusters to Polarized Sources

<table>Simulated patches of the sky at 100, 143, 217, 353, 545 and 857 GHz. A bright galaxy cluster is in the centre of the patches, but it is almost invisible among the CMB and Galaxy fluctuations.</table>

Advances in Astronomy

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Figure 3

Figure 3: Compact Source Detection in Multichannel Microwave Surveys: From SZ Clusters to Polarized Sources 