Fig. 11.
Median SSFR as a function of redshift with a 68% confidence limit based on the whole PDF with comparison of results from different studies (Noeske et al. 2007; Daddi et al. 2007; Reddy et al. 2012) and results from the study of de Barros et al. (2014, DB14) for four different models. The dashed line shows the relation expected from Bouché et al. (2010) for an exponentially increasing star formation at a fixed stellar mass, 109.5 M⊙.
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