Fig. 2
Measurements of the CIB auto- and cross-power spectra obtained by Planck and IRAS (extracted from Planck Collaboration XXX 2014) and the best fit CIB linear model. Data points on higher ℓ are not shown as they are not used for fitting. We also show the shot noise (black dash-dotted line) and one-halo term (red dashed line) for all the frequencies.
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