Fig. 3
The same as Fig. 2 but for the M 31 halo (temperature contrast of the N1+S1 with respect to the N2+S2 regions in mK/pixel – red line) for 500 random control fields (continuous lines) and 500 simulated sky maps (dashed lines). Here the WMAP maps with the Galactic disk contribution modeled and removed (foreground-reduced maps) are used.
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