Fig. E.4
CMB TT (left) and EE (right) power spectra for each of the four foreground-cleaned CMB maps. Upper panels show raw band-powers; the grey lines show the best-fit ΛCDM model from the Planck 2015 likelihood. Lower panels show residual band-powers after subtracting the best-fit ΛCDM model, showing the residual extragalactic foreground contribution.
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