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Table C.5.

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
(mag) (mag) (M yr−1) (yr−1)
071112C −18.49 0.15 2.11
111228A −18.57 0.40 0.01
120714B −18.33 0.08 0.01
130831A −17.72 0.02 0.55

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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