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Fig. A.4
Dust EE, BB, and TE
cross-power spectra in units of 
computed from the subsets of 100 realisations of the dust model maps over mask65 using the CNM, LNM, and WNM of KH18 and the fourth template. The filled areas represent the Planck dust power spectra measurements over mask65 computed in Sect. 4.3.
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