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Fig. 17


UV extinction vs. stellar mass diagram. Plotted with the average relation and standard deviation obtained with the GOODS-Herschel sample by Buat et al. (2012) in the redshift range 0.9 < z < 2.2, after correcting it with a factor of 1.8 to account for the difference in the choice of IMFs. Also plotted is the relation from Pannella et al. (2009) for a sample of radio observed BzKs. The values shown with black diamonds are derived from the observed IR-to-UV ratio via the correspondence from Schaerer et al. (2013).

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