Fig. 10
This figure illustrates the ratio between the observed fluxes at 24 μm and 70 μm as a function of the Ldust estimated by the code. The solid red line corresponds to the results given by the DH02 templates at z = 0.7. The dashed cyan line is given by Siebenmorgen et al. (2004b) for typical AGN contaminated object. AGNs described in Sect. 4.2 are shown as red stars.
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