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Fig. 6

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Same as Fig. 5, but using the regions defined in DF08. Clearly, the residuals near the mask are significantly reduced, although, as with the full-sky fits, striping in the HFI channels (which leaks into the CMB estimate) becomes significant above ~40 GHz.

This figure is made of several images, please see below:
thumbnail Open with DEXTER Download original image
thumbnail Open with DEXTER Download original image
thumbnail Open with DEXTER Download original image
thumbnail Open with DEXTER Download original image
thumbnail Open with DEXTER Download original image
thumbnail Open with DEXTER Download original image

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