Fig. 18

Effect of adopting an age prior (minimum age t > 50 Myr) on the predicted IR luminosity for declining (green, model A) and rising (red, model D) histories. We plot the difference in log (LIR) between the unconstrained model and the one with age prior as a function of the latter. On average declining SFH show lower LIRwhereas rising histories predict basically the same, or even higher IR luminosities. Rising SFHs case can thus be distinguished from constant SFR, even if age priors apply.
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