Fig. 2.
Examples of SED fit with 
= 1.24 (left), 
= 2.37 (middle), and 
= 6.39 (right). The best model from CIGALE SED fitting is shown in solid line. The observed fluxes (open circles), the model spectrum of the stellar population (dashed line), the model fluxes (dots), and the dust emission (dotted line) are overplotted. For the fit with 
> 5 (right), the discrepancy between the observed fluxes and the best model is significant.
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