Open Access
Table A.3.
Stellar masses for the hosts of the BAT6 LGRB sample at 2 < z < 3.
| Name | Redshift | log(M*/M⊙) | Mref |
|---|---|---|---|
| 070328 | 2.0627 | 10.0 | 2 |
| 090201 | 2.1000 | 10.9 | 1 |
| 100728B | 2.106 | <9.3 | 2 |
| 050922C | 2.1995 | <9.0 | 2 |
| 080804 | 2.2059 | 9.3 | 2 |
| 081221 | 2.2590 | 10.8 | 2 |
| 090812 | 2.452 | <9.4 | 2 |
| 081121 | 2.512 | 9.2 | 2 |
| 080721 | 2.5914 | <9.6 | 2 |
| 081222 | 2.77 | 9.6 | 2 |
| 050401 | 2.8983 | 9.6 | 2 |
Notes. The galaxy stellar masses are computed using only the NIR Spitzer/IRAC1 magnitudes or limits (Perley et al. 2016b; see Sect. 2.2). References. (1) This work; (2) Perley et al. (2016b).
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