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Table 2.

Rest-frame SGRB sample.

GRB GBM name T90/s z Redshift source (⋆)
080905A GRB080905499 0.960 ± 0.345 0.1218 ± 0.0003 Fong et al. (2022; Gold)
090510 GRB090510016 0.960 ± 0.138 0.903 ± 0.002 Rau et al. (2009), Levan (2009)
100117A GRB100117879 0.256 ± 0.834 0.914 ± 0.0004 Fong et al. (2022; Gold)
100206A GRB100206563 0.176 ± 0.072 0.40 ± 0.002 Fong et al. (2022; Gold)
100625A GRB100625773 0.240 ± 0.276 0.452±0.002 Fong et al. (2022; Silver)
111117A GRB111117510 0.432 ± 0.082 2.211 ± 0.001 Fong et al. (2022; Silver)
130515A GRB130515056 0.256 ± 0.091 0.80 ± 0.01 Fong et al. (2022; Silver)
130912A GRB130912358 0.512 ± 0.143 N/A
131004A GRB131004904 1.152 ± 0.590 0.717 ± 0.002 Fong et al. (2022; Silver)
160821B GRB160821937 1.088 ± 0.977 0.1619 ± 0.0002 Fong et al. (2022; Silver)
170127B GRB170127634 1.728 ± 1.346 2.28 ± 0.14 (⋆ ⋆) Fong et al. (2022; Silver)
180204A GRB180204109 1.152 ± 0.091 N/A
180727A GRB180727594 0.896 ± 0.286 (⋆ ⋆) Fong et al. (2022; Gold)
191031D GRB191031891 0.256 ± 0.023 (⋆ ⋆) Fong et al. (2022; Silver)
200219A GRB200219317 1.152 ± 1.032 0.48 ± 0.02 Fong et al. (2022; Gold)
200411A GRB200411187 1.440 ± 0.506 (⋆ ⋆) Fong et al. (2022; Bronze)
201221D GRB201221963 0.144 ± 0.066 1.046 ± 0.002 de Ugarte Postigo et al. (2020)
210323A GRB210323918 0.960 ± 0.781 0.733 ± 0.001 Fong et al. (2022; Gold)

Notes. The sample consists of SGRBs belonging to the extended S-BAT4 sample (original sample: D’Avanzo et al. 2014; extended sample: Ferro et al. 2023, D’Avanzo et al., in prep.) and also detected by Fermi/GBM with T90 < 2 s. (⋆)Fong et al. (2022) host galaxy class in parentheses, where available, based on the probability Pcc of a chance association with the SGRB. Gold: Pcc ≤ 0.02; Silver: 0.02 < Pcc ≤ 0.1; Bronze: 0.1 < Pcc ≤ 0.2. (⋆ ⋆)Photometric redshift posterior samples retrieved from the BRIGHT online catalogue at https://bright.ciera.northwestern.edu/.

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