Fig. 16

Pseudo-power spectra for TE (left) and TB (right) for each frequency (from top to bottom: 100, 143, 217, and 353 GHz). The auto-spectra are shown in black. Cross-spectra of half-ring (HR), half-mission (HM), and detector-set (DS) half-differences are shown in blue, red, and green, respectively. A Galaxy and point source mask, leaving 40% of the sky, was used in all cases.
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