Fig. 6
Templates of the dipole and the Galaxy, in MJy/sr, seen through our far sidelobes for Surveys 1 (left) and 2 (centre), and for the difference in these two (right). Row 1: dipole seen through the direct SR contribution. Row 2: dipole seen through the PR contribution. Row 3: dipole seen through the baffle SR contribution. Row 4: galaxy seen through the direct SR contribution. Row 5: galaxy seen through the PR contribution. Row 6: galaxy seen through the baffle SR contribution. The simulations in Rows 4–6 are made using 857 GHz data passed through the far sidelobe calculation described in Sect. 4.2. The scales are different for the top and bottom three rows, and for the first two and the last columns.
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