Table A.1.
GRB for which the extinction curves are derived by fitting with the FM formula in Zafar et al. (2011, 2012).
| GRB | z | TSED |
|
Ext. curve | pow/bknp |  |
log10 M⊙ |  |
SFRHα | Z | References |
|---|---|---|---|---|---|---|---|---|---|---|---|
| h | mag | mag | mag | M⊙ yr−1 | 12 + log(O/H) | ||||||
| 050401 | 2.8983 | 14.7 | 0.172 | SMC-like | bknp |
|
9.61 | (1), (4) | |||
| 060729 | 0.5428 | 13.2 | 0.142 | SMC-like | pow |
|
8.31 |
|
|
(1), (4), (5) | |
| 070125 | 1.5471 | 31.5 | 0.139 | SMC-like | bknp |
|
(1) | ||||
| 070802 | 2.4541 | 2.00 | 0.071 | LMC-like | pow |
|
|
|
(1), (5) | ||
| 071020 | 2.1462 | 5.12 | 0.160 | SMC-like | bknp |
|
<9.43 | (1), (4) | |||
| 080605 | 1.6403 | 1.74 | 0.360 | Steep + bump | pow |
|
10.53 |
|
|
|
(2), (4), (5) |
| 080607 | 3.0368 | 0.08 | 0.185 | Flat + bump | pow |
|
10.45 | (1), (4) | |||
| 080805 | 1.5042 | 1.00 | 0.114 | Flat + bump | pow |
|
9.86 |
|
|
|
(2), (4), (5) |
| 080928 | 1.6919 | 15.5 | 0.179 | SMC-like | pow |
|
<9.29 | (1), (4) | |||
| 120119A | 1.728 | 1.77 | 0.295 | SMC | pow |
|
9.91 |
|
|
|
(3), (4), (5) |
Notes.The GRBs in bold are the ones in our Golden sample. Columns list (1) the redshift, (2) time at which the SED is extracted, (3) the Galactic extinction, (4) type of extinction curve, (5) whether the GRB afterglow SED is best fitted with a power law or broken power law, (6) the amount of extinction in the V band along the GRB l.o.s. in the host galaxy, (7) stellar mass of the GRB host galaxy from Perley et al. (2016), (8) amount of extinction in the host galaxy derived from the Balmer decrement, (9) the SFR derived from Hα luminosity, (10) the metallicity, (11) references where these quantities are found.
References. Zafar et al. (2011; 2) Zafar et al. (2012; 3) Zafar et al. (2018; 4) Perley et al. (2016; 5) Krühler et al. (2015).
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