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Fig. 20


Average full-sky spectra of noise residual maps after the destriping and calibration pipeline for the datasets: pure white noise, and low frequency noise plus white noise with fknee = 0.1 Hz and 0.01 Hz. The effect of the calibration uncertainty is represented by the spectra of the residual map constructed using estimated gains (blue dashed line). The simulation power spectra and CMB WMAP-5yr fiducial model are also plotted for comparison. Upper line, from left to right: temperature, E-mode, B-mode. Bottom line, from left to right: cross-correlation TE, TB, and EB.

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