Spectra of Archeops compact sources (diamonds), binned in temperature, fitted using the TLS model, with the best-fit parameters (this page) and the standard parameters (next page). The contribution of the different processes is given in the caption of Fig. 2. Squares correspond to the model after color correction. The average temperature per bin deduced from a single modified black-body fit (from Désert et al. 2008), and the temperature deduced from the TLS model are given in the top right of each panel. The description of the Archeops spectra is given in Sect. 2.2 and in Table 2.