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Fig. B.1


Examples of galaxies fitted with the standard approach (“free AV”, cyan), and with the energy conserving approach (“fixed AV”, red). The photometry is shown with blue circles, and the error bars are 1σ. For each fit, we show the reduced and the ratio of predicted over observed LIR (ΔIR = log (LIR,predicted/LIR,observed)). Although in some cases the “before and after” SEDs look similar in first order, they can represent different sets of parameters, illustrating how the LIR constrain helps in finding solutions that are more consistent with the observations.

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