Table 5
New GRB redshifts.
| GRB host | Redshift | Spectral features |
|
|
||
| GRB 050714B | 2.4383 | [O iii](5007), Hα |
| GRB 060306a | 1.5585/1.5597 | [O ii], Hα |
| GRB 060805Ab | 2.3633 | Hβ, [O iii](5007), Hα |
| GRB 060923B | 1.5094 | [O iii](5007), Hα |
| GRB 070224 | 1.9922 | [O iii](4959,5007) |
| GRB 070328 | 2.0627 | [O ii], Hβ, [O iii] |
|
|
||
| GRB 070521 | 2.0865 | Hα |
| GRB 080602 | 1.8204 | [O ii], [O iii], Hα |
| GRB 090201 | 2.1000 | [O ii], Hβ, [O iii], Hα |
|
|
||
| GRB 100508A | 0.5201 | [O ii], Hβ, [O iii], Hα |
| GRB 111129A | 1.0796 | [O ii] |
| GRB 120211A | 2.4 ± 0.1 | Ly-α break |
| GRB 120224A | 1.1 ± 0.2 | Balmer break |
| GRB 120805A | 3.1 ± 0.1 | Ly-α break |
| GRB 121209A | 2.1 ± 0.3 | Balmer break |
| GRB 140114A | 3.0 ± 0.1 | Ly-α break |
Notes. The horizontal lines denote the separation between TOUGH GRBs (upper part), BAT6 (middle part) and others.
Emission lines of the host of GRB 060306 have a double-peaked profile, and we thus provide two redshifts.
Ambiguous association because two galaxies are present in the XRT error-circle. This is the redshift for the fainter of the two objects, for details see Jakobsson et al. (2012).
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