Fig. A.3.
Top panel: Commander CMB temperature map used for the Planck low-ℓ temperature likelihood analysis, smoothed to 60′ FWHM resolution. The grey region indicates the mask adopted for the likelihood analysis, which retains 86% of the sky. Bottom panel: difference between the low-ℓ likelihood and full-resolution Commander CMB temperature maps, smoothed to 60′ FWHM resolution.
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