Planck 2013 results
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Fig. 16


CMB multipole spectrum residuals for best fit primordial power spectrum reconstruction with smoothing parameter λ = 103. The panels show the C spectrum residuals (compared to the best fit power law fiducial model represented by the horizontal straight dashed line) for the four auto- and cross-spectra included in the high- likelihood. Here The data points have been binned with Δ = 31 and foregrounds subtracted according to the best fit foreground parameters. The solid black line shows the CMB spectrum residual for the maximum likelihood primordial power spectrum reconstruction with λ = 103.

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