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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 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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