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Lack of large-angle TT correlations persists in WMAP and Planck

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Academic year: 2021

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Figure 1. Two-point angular correlation function from the inpainted Planck SMICA map. The black, dotted line shows the best-fitting CDM model from Planck
Table 2. Same as Table 1 now with the DQ-corrected maps.
Figure 2. Masks used in this work. A pixel may be removed by both masks (dark blue), only the KQ75y9 mask (light blue), only the U74 mask (yellow), or by neither mask (red).
Figure 4. Cut-sky C ( θ ) using the KQ75y9 mask for individual frequency band maps. Shown are correlation functions from the WMAP nine-year W (black, solid line) and V (red, dashed line) bands along with the Planck HFI 100 GHz (green, dash–dotted line) and

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