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Fig. C.1.
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IR inferred SFRs versus time-averaged SFR over 100 Myr for NEWCLUSTER (squares) and NEWHORIZON (circles) simulated galaxies. We color code the data points based on the ratio of the total IR (8 − 1000 μm) and far-UV (1500 Å) luminosity (see Sect. 4.2 for details).
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