Open Access

Fig. 1.


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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.