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Fig. B.3


A selection among the sources for which the energy conserving approach does not produce good quality fits. We recall that those sources lie on the high LIR end, and have bluer slopes than what is inferred by their IRX ratios. As a consequence, the difference between the free and fixed AV solutions are significant. While the unconstrained fits (cyan) range from moderately good to very good, they underpredict the LIR by more than 1 dex. The fixed AV fits (red) present SEDs that are incompatible with the photometry, and in cases still do not account well for the LIR. Colors and symbols as in B.1.

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