Table A.2.
GRB extinction curves derived by scaling the LMC, SMC and MW extinction curves of Pei (1992).
| GRB | z | TSED |
|
Ext. curve | pow/bknp |  |
log10 M⊙ |  |
SFRHα | Z | References |
|---|---|---|---|---|---|---|---|---|---|---|---|
| h | mag | mag | mag | M⊙ yr−1 | 12 + log(O/H) | ||||||
| 050820A | 2.615 | 2.78 | 0.14 | LMC | bknp |
|
9.38 | (3), (1) | |||
| 060418 | 1.49 | 1.39 | 0.69 | SMC | bknp |
|
(3) | ||||
| 060607A | 3.082 | 2.22 | 0.09 | SMC | pow |
|
<9.45 | (3), (1) | |||
| 060904B | 0.703 | 1.39 | 0.53 | LMC | pow |
|
(3) | ||||
| 061121 | 1.314 | 1.67 | 0.14 | LMC | bknp |
|
10.31 |
|
|
|
(3), (1), (4) |
| 071112C | 0.823 | 0.36 | 0.36 | SMC | pow |
|
8.89 | <0.2 |
|
(3), (1), (5) | |
| 080210 | 2.641 | 1.39 | 0.26 | LMC | bknp |
|
<9.50 | (3), (1) | |||
| 080319C | 1.95 | 0.14 | 0.08 | SMC | pow |
|
(3) | ||||
| 080710 | 0.845 | 2.78 | 0.23 | SMC | pow |
|
<8.95 | (3), (1) | |||
| 080804 | 2.204 | 0.42 | 0.05 | LMC | bknp |
|
9.28 |
|
|
(3), (1), (2) | |
| 081121 | 2.512 | 2.77 | 0.16 | SMC | bknp |
|
9.24 | (3), (1) | |||
| 081222 | 2.77 | 0.19 | 0.06 | MW | bknp |
|
9.61 | (3), (1) | |||
| 090102 | 1.546 | 0.28 | 0.15 | MW | bknp |
|
(3) | ||||
| 090424 | 0.544 | 0.28 | 0.08 | MW | bknp |
|
9.62 |
|
|
|
(3), (1), (5) |
| 090618 | 0.54 | 0.55 | 0.27 | SMC | bknp |
|
9.04 | (3), (1) | |||
| 091018 | 0.971 | 8.33 | 0.09 | SMC | bknp |
|
9.62 |
|
|
|
(3), (1), (2) |
| 091029 | 2.752 | 0.28 | 0.05 | LMC | bknp |
|
<9.81 | (3), (1) | |||
| 100814A | 1.44 | 98.4 | 0.054 | SMC | bknp |
|
9.52 |
|
|
(6), (1), (2) | |
| 100901A | 1.408 | 66.0 | 0.270 | SMC | bknp |
|
(6) | ||||
| 120815A | 2.358 | 2.06 | 0.320 | SMC | bknp |
|
|
|
(6), (1), (2) |
Notes. GRBs of the upper part of the table are taken from Schady et al. (2012), GRBs in the lower part are taken from Japelj et al. (2015). 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 tracer, (10) the SFR derived from Hα luminosity, (11) the metallicity, (12) references where these quantities are found.
References.(1) Perley et al. (2016; 2) Krühler et al. (2015; 3) Schady et al. (2012; 4) Vergani et al. (2017; 5) Japelj et al. (2016; 6) Japelj et al. (2015).
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