Fig. 44.
Comparison between the dust contribution to the EE power spectra, as estimated from the “dust cleaning” procedure in Eq. (32) (dashed lines), and the smooth power-law model used in the likelihood (solid lines). The data points are the 100 × 100, 143 × 143, and 217 × 217 spectra (from top to bottom) minus the best-fit Planck baseline 2018 results (shown in dot-dashed grey).
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