Planck 2018 results
Open Access

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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