Fig. 15
Redshift contribution to the Cℓ at several wavelengths using our emissivities on the left and using Lagache et al. (2004) emissivity on the right. In both cases, the contribution of high redshift increases with the wavelength but the evolution goes faster with Lagache et al. (2004) emissivities. These redshift distributions are strongly varying with the halo parameters (see Fig. 10).
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