Fig. 9
α parameter estimated with CIGALE as a function of the 60 to 100 μm flux ratio, R(60, 100) for galaxies observed at all far-IR wavelengths, up to 160 μm. Vertical error bars represent the standard deviation in the determination of α given by the Bayesian analysis. The relation between α and R(60, 100) for the DH02 models is plotted as a solid line.
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