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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