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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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