Fig. 12
GNILC CIB maps for a large fraction of the sky at 353 GHz (top), 545 GHz (middle), and 857 GHz (bottom). Apart from thermal dust reconstruction, the GNILC component-separation method gives access to CIB anisotropies over 57% of the sky. The left panels show the GNILC CIB maps at full resolution while the right panels show the CIB maps smoothed to one degree resolution.
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