Fig. 12
Correlation between the 143 and 857 GHz frequency maps on 28% of the sky (Hi column density smoothed at 1° lower than 3 × 1020 cm-2). CMB anisotropies have been removed at 143 GHz. Left: raw correlation. Right: correlation after a residual solar dipole has been removed at 143 GHz. The offset of this correlation sets the Galactic zero level of the 143 GHz map.
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