Advances in High Energy Physics / 2013 / Article / Fig 2

Research Article

Cosmic Dark Radiation and Neutrinos

Figure 2

CMB temperature power spectrum. The model and the legend are the same as in Figure 1, the grey error bars correspond to Planck data. (a) The total CMB temperature power spectrum. (b) The axis has been rescaled by a factor . (c) The total contribution has been subtracted. (d) The total ISW (both the autocorrelation and the cross correlation) contribution have been subtracted.

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