Fig. 11.
SSFR vs. stellar mass for a sample of GRB hosts, inferred from template fitting to their photometric SEDs. The host of GRB 140629A is shown by a green star. Black dots indicate burst hosts with SFRs measured from GHostS from 1997 to 2014 (Savaglio et al. 2006, 2009). The dashed lines indicate the constant SFRs of 0.1, 1, 10, and 100 M⊙ yr−1 from left to right.
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