Fig. 10
Specific SFR as a function of redshift. The sSFR of our sample, Ono et al. (2010), Mallery et al. (2012), and Wofford et al. (2013) is calculated using only SED fitting, for Hayes et al. (2014), Henry et al. (2015) the sSFR is calculated using the SFR based on Hα, and the sSFR of Jiang et al. (2016) is calculated using SFRUV. The black line shows the sSFR of the CANDELS galaxies from Salmon et al. (2015).
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