Planck 2015 results
Free Access

Fig. 26

image

Correlated noise model. In grey are shown the cross-detector TT spectra of the half-ring difference maps. The black line show the same, smoothed by a Δ = 200 sliding average, while the blue data points are a Δ = 100 binned version of the grey line. Error bars simply reflect the scatter in each bin. The green line is the spline-smoothed version of the data that we use as our correlated noise template.

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