Fig. 6
Left panel: dust EE, BB, and TE cross-power spectra computed from the subsets of Planck data at 353 GHz over mask65. Dashed lines represent the best-fit power laws. Right panel: similar plots as left panel computed from 100 realisations of the dust model maps. Error bars are 1 σ uncertainties as explained in the main text. The filled areas represent the Planck dust power spectra measurements over mask65.
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