Planck 2015 results
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Fig. 48

image

Comparison of Planck and WMAP-9 CMB power spectra. Top: direct comparison. Noise spectra are derived from the half-ring difference maps. Bottom: residuals with respect to the PlanckΛCDM best-fit model. The error bars do not include the cosmic variance contribution (but the (brown) 1σ contour lines for the Likelihood best fit model do).

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