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Fig. 1.

image

Angular power auto-spectra of the clustered CIB component used in simulations. The dashed lines represent the 1D clustered CIB spectra obtained by fitting data points to a polynomial at 545 GHz and scaling this template to lower frequencies. The solid lines represent the ND clustered CIB obtained by separately fitting data points at each frequency. Overplotted data are taken from Table D2 of Planck Collaboration XXX (2014). No data points are available for the 100 GHz clustered spectrum, which is taken to be one order of magnitude less than the 143 GHz clustered spectrum. Spectra have been corrected for shot-noise contribution in order to match data points.

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