Figure 5 from Fast and Optimal Cosmic Microwave Background Lensing Using Statistical Interpolation on the Sphere

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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 5.

Accuracy of the error estimate. The thick black line shows the measured error normalized using the error estimate, Equation (16), at each pixel. The overplotted thin red line is a Gaussian distribution of width 1 and centered on 0 showing perfect agreement between the predicted and actual errors.

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