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Table A.4.
Measured line fluxes in units of 10−17 erg s−1 cm−2, corrected for Galactic foreground extinction.
| Name | Redshift | [O II] λ3726 | [O II] λ3729 | [Ne III] λ3868 | Hγ | Hβ | [O III] λ4959 | [O III] λ5007 | Hα | [N II] λ6583 | Ref. |
|---|---|---|---|---|---|---|---|---|---|---|---|
| GRB050318 | 1.4436 | - | |||||||||
| GRB050802 | 1.7117 | 1.7 ± 0.4 | 2 | ||||||||
| GRB060306 | 1.5597 | 0.7 ± 0.4 | 1.0 ± 0.3 | 1.1 ± 1.4 | 1.4 ± 2.0 | 3.3 ± 4.6 | 8.9 ± 3.7 | 2.4 ± 1.4 | 1 | ||
| GRB060814 | 1.9223 | 26.3 ± 3.7a | 8.3 ± 3.4 | 8.4 ± 1.8 | 31. ± 7.8 | 28.0 ± 5.7 | 1 | ||||
| GRB060908 | 1.8836 | 2 | |||||||||
| GRB061007 | 1.2623 | 2.4 ± 0.3a | <2.0 | 1.0 ± 0.4 | 9.5 ± 1.4 | 4.0 ± 0.4 | <2.4 | 2 | |||
| GRB061121 | 1.3160 | 8.3 ± 1.1 | 18.4 ± 1.1 | 2.5 ± 0.5 | 4.2 ± 1.4 | 7.9 ± 1.6 | 7.9 ± 1.6 | 26.6 ± 1.4 | 40.0 ± 0.9 | 4.5 ± 0.8 | 2 |
| GRB070306 | 1.4965 | 9.1 ± 0.7 | 7.7 ± 0.7 | 1.9 ± 0.4 | 7.7 ± 3.7 | 11.6 ± 1.4 | 15.5 ± 1.3 | 46.0 ± 3.6 | 53.5 ± 4.0 | 6.4 ± 0.4 | 1 |
| GRB071117 | 1.3293 | 2.0 ± 0.3 | 3.4 ± 0.3 | <0.4 | 3.0 ± 0.6 | 6.6 ± 1.1 | 5.6 ± 1.0 | <1.2 | 2 | ||
| GRB080413B | 1.1012 | 0.6 ± 0.2 | 0.8 ± 0.2 | 0.2 ± 0.2 | 0.2 ± 0.2 | 2.8 ± 0.9 | 2.6 ± 1.3 | 1 | |||
| GRB080602 | 1.8204 | 28. ± 4.0a | 21.7 ± 4.0 | 43.7 ± 5.0 | 2 | ||||||
| GRB080605 | 1.6408 | 7.9 ± 1.1 | 9.2 ± 1.5 | 7.7 ± 1.5 | 10.3 ± 1.6 | 29.6 ± 4.6 | 29.1 ± 4.5 | 4.0 ± 0.7 | 1 | ||
| GRB090926B | 1.2427 | 4.8 ± 0.8 | 7.1 ± 0.8 | <2.2 | <2.8 | 2.4 ± 1.2 | 3.1 ± 1.0 | 12.2 ± 1.5 | 11.5 ± 1.2 | <3.0 | 2 |
| GRB091208B | 1.0633 | - | |||||||||
| GRB100615A | 1.3979 | 1.8 ± 0.6 | 2.7 ± 0.6 | 1 ± 0.3 | <3.0 | <2.8 | 6.4 ± 1.1 | <1.6 | 2 |
Notes.
(a)
Cases where the [O II] doublet is not resolved. The total integrated flux is reported in this column.
References. (1) Krühler et al. (2015); (2) this work.
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