Fig. 10.
Redshift evolution of the sSFR. Results of various observations and numerical simulations are shown. The magenta star shows the result of this work, an extension of Tasca et al. (2015) work (light blue stars). The solid line shows the fit to the previous results from VUDS (Tasca et al. 2015), the shaded area and the dashed line shows the results, coming from the observations of EW(Hα) in COSMOS (Faisst et al. 2016).
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