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Fig. 2.
CMB-corrected EE (red diamonds), BB (blue squares), and TE (black circles) power spectra at 353 GHz, for each of the six sky regions that we analyse. The dashed lines represent power-law fits to the data points from ℓ = 40 to 600. The exponents of these fits, αTE, αEE, and αBB, appear on each panel.
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