Planck 2013 results
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Fig. 6

image

Relative contributions of CMB, instrumental noise, and foreground power terms discussed in Sect 5.1 to the approximate lens reconstruction variance of Eq. (21), previously plotted in Fig. 1. As discussed in Sect. 5.1, the finite number of CMB modes observed by Planck is the dominant source of variance for the lens reconstruction.

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