Fig. 4

Simulation of the Wiener-filtered lensing potential estimate
for the MV reconstruction
(left), and the input φ realization (right; filtered
by
to be directly comparable to the
Wiener estimate). Both maps show the southern Galactic sky in orthographic projection.
The lensing reconstruction is noise dominated on all scales, however correlations
between the two maps can still be seen visually.
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