Fig. 18
Wiener-filtered lensing potential estimate, in Galactic coordinates using orthographic projection (Planck Collaboration XVII 2014). The reconstruction was bandpass filtered to L ∈ [10,2048]. Note that the lensing reconstruction, while highly statistically significant, is still noise dominated for every individual mode, and is at best S/N ≈ 0.7 around L = 30.
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