Dust-plus-CIB contamination estimates in temperature. The 100 × 100, 143 × 143, and 217 × 217 half-mission cross-spectra with the 2018 Planck CMB best-fit subtracted are shown from top to bottom. The green line shows , with the aν rescaling factor estimated from Eq. (29), the black line shows , while the dotted coloured line shows the dust contribution as estimated from the cleaning procedure in Eq. (32). The grey dotted line shows the TT CMB best-fit.
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