Fig. 7
Maps of the effect from far sidelobes. Rows correspond to 30, 44, and 70GHz channels, while columns correspond to I, Q, and U. The straylight signal at 30GHz is larger compared to 44 and 70GHz. The 44GHz channel is the least contaminated by this effect. This behaviour results from the combination of the beam far sidelobes and the intensity of the Galactic emissions at the LFI frequencies.
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