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Fig. 7.


IRX–AFUV relation derived from a sample of star-forming galaxies extracted at z = 1.5. The gray solid line indicates our best fit. For comparison we also plot the Buat et al. (2005) best fit (black solid line). Colored points show a subsample that is uniformly selected in the IRX–AFUV plan. The color scale shows the luminosity-weighted age of the stellar population hosted by the galaxy.

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