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Fig. 3


Noise residual full-sky power spectra with various internal Galactic mask applied to the offset determination. Residual maps are at nside = 1024. Spectra are smoothed over five multipoles. Signal spectra are plotted in red. As a reference, we also plot the CMB WMAP five-year fiducial model (black) and a total power of the simulated sky signal, CMB+Galaxy+noise, (red curve). From left to right: temperature, E-mode, and B-mode.

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