Fig. 4
Linear part (top panel) and non-linear correction (bottom panel) for a non-Gaussian CMB realisation, at 1° resolution. Note the different colour scales, and that fNL ~ 1 (or a few) is a typical expected level. The cosmological parameters assumed for this simulation are from the fit of WMAP 7-year + BAO + SN observations, as made available on the LAMBDA web site.
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