Fig. 13
Wiener-filtered lensing potential estimate with minimal masking (using the SMICA component-separated map), in Mollweide projection in Galactic coordinates (Planck Collaboration XV 2016). The reconstruction has been band-limited to 8 ≤ L ≤ 2048 (where, following convention, L is used as the multipole index in the lensing power spectrum).
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