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Fast and Optimal Cosmic Microwave Background Lensing Using Statistical Interpolation on the Sphere

  • Authors: Guilhem Lavaux and Benjamin D. Wandelt

LAVAUX & WANDELT 2010 The Astrophysical Journal Supplement Series 191 32.

  • Provider: AAS Journals

Caption: Figure 3.

Spatial distribution of predicted interpolation error for the upsampling. We show the distribution of the error predicted by the algorithm for each interpolated pixel of the sky. We predict a map at N side = 4096 from a map at N side/2= 2048, with ℓ max = 4096. The structure of the error distribution reflects the features of the HealPix pixelization.

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