Results of the stellar population synthesis fits using Le PHARE and adopting a starburst model.
|GRB||MB||E(B − V)host||log SFR||log M/M⊙||logsSFR||χ2|
|Median values of the unbiased Swift/BAT6 GRB host galaxy sample at z < 1 from Vergani et al. (2015)|
|Median values of the z < 0.5 GRB host galaxy sample from Schulze et al. (2018)|
|−18.33 ± 0.41||...||−0.19 ± 0.13||8.83 ± 0.20||−9.15 ± 0.11||...|
Notes. The integrated host properties were derived by fitting the SED of the host galaxies with stellar-population-synthesis models by Bruzual & Charlot (2003) in Le PHARE. The SEDs of the BAT6 sub-sample were fitted using the same method. The errors of the median values indicate the distance to the 16 and 84%-iles.
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