Fig. 4
GNILC dust maps at 353 GHz (left panel), 545 GHz (middle panel), and 857 GHz (right panel) on a 
gnomonic projection of the sky centred at high latitude, (l,b) = (90°,−80°). GNILC filters out the CIB anisotropies while preserving the small-scale dust signal (see bottom panel of Fig. 2). In these images, the local mean intensity of each map has been subtracted.
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