Fig. 14
Ratios of 100, 143, and 217 GHz power spectra calculated from detector sets with the likelihood method, including subtraction of the best-fitting foreground model (see text) and correction for the best-fit relative calibration factors for individual detectors. Solid symbols and lines show ratios for mask G22; open symbols and dotted or dashed lines show ratios for mask G35. The greater scatter in 217/143 for mask G35 is caused by CMB-foreground cross-correlations.
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