Fig. B.1
Set of unapodised foreground masks, G22, G35, G45, G56, G65, PS96, which, once apodised, are used for the likelihood analyses. The Galactic (G22 to G65) masks are defined using a threshold of the 353 GHz Planck temperature map. The (lower-right) PS96 point source mask is based on the union of resolved sources in all channels from 100 GHz to 353 GHz.
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