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Table 3

Fluxes of forbidden lines for GRB hosts.

GRB host Redshift [O ii] [Ne iii] [O iii] [N ii]
λ3726 λ3729 λ3869 λ4959 λ5007 λ6584
GRB 050416A 0.6542 4.9 ± 0.4 ± 0.5 4.5 ± 0.5 ± 0.4 0.7 ± 0.4 ± 0.1 2.5 ± 0.3 ± 0.3 7.8 ± 0.6 ± 0.8 1.9 ± 0.6 ± 0.2
GRB 050525Ab 0.6063 0.2 ± 0.2 ± 0.2 0.1 ± 0.1 ± 0.1 0.4 ± 0.1 ± 0.2 0.8 ± 0.1 ± 0.3 − 0.2 ± 0.3 ± 0.1
GRB 050714Bb 2.4383 2.2 ± 1.0 ± 0.5 0.1 ± 0.3 ± 0.1 0.0 ± 0.3 ± 0.1 1.0 ± 0.4 ± 0.3 − 1.4 ± 0.6 ± 0.1
GRB 050819A 2.5042 1.0 ± 0.5 ± 0.2 1.4 ± 0.4 ± 0.3 ··· ··· 5.2 ± 0.7 ± 0.9 − 1.9 ± 0.8 ± 0.2
GRB 050824 0.8277 2.0 ± 0.2 ± 0.4 2.6 ± 0.2 ± 0.5 1.1 ± 0.1 ± 0.2 6.5 ± 0.3 ± 1.3 18.5 ± 0.8 ± 3.6 0.3 ± 1.0 ± 0.1
GRB 050915Ab 2.5275 3.0 ± 0.5 ± 0.5 ··· 1.0 ± 0.1 ± 0.2 2.9 ± 0.5 ± 0.6 ···
GRB 051001b 2.4295 4.6 ± 2.0 ± 0.8 1.0 ± 0.5 ± 0.2 − 0.3 ± 0.6 ± 0.1 5.3 ± 0.8 ± 1.0 − 3.0 ± 1.5 ± 0.2
GRB 051016B 0.9358 13.0 ± 0.6 ± 1.2 15.6 ± 0.7 ± 1.4 3.7 ± 0.4 ± 0.3 15.9 ± 1.1 ± 1.5 53 ± 2 ± 5 ···
GRB 051022A 0.8061 23.2 ± 1.2 ± 1.8 30.9 ± 1.2 ± 2.4 4.1 ± 0.8 ± 0.4 21.3 ± 1.3 ± 1.7 63 ± 2 ± 5 17 ± 3 ± 3
GRB 051117B 0.4805 1.4 ± 0.7 ± 0.1 1.7 ± 1.0 ± 0.1 − 1.0 ± 1.2 ± 0.1 1.1 ± 1.3 ± 0.1 1.2 ± 0.9 ± 0.1 7.1 ± 1.6 ± 0.4
GRB 060204B 2.3393 5.6 ± 0.5 ± 0.7 3.8 ± 0.5 ± 0.5 1.2 ± 0.9 ± 0.3 5.7 ± 0.6 ± 0.8 16.9 ± 1.4 ± 2.2 0.7 ± 0.8 ± 0.2
GRB 060306 1.5597 0.7 ± 0.3 ± 0.1 1.0 ± 0.2 ± 0.1 1.1 ± 1.4 ± 0.3 ··· 3.3 ± 4.5 ± 0.9 2.4 ± 1.4 ± 0.4
GRB 060604b 2.1355 0.5 ± 0.5 ± 0.2 ··· 1.0 ± 0.2 ± 0.3 4.0 ± 0.3 ± 0.9 ···
GRB 060707b 3.4246 1.8 ± 1.0 ± 0.6 ··· − 0.4 ± 2.0 ± 0.4 4 ± 4 ± 2 ···
GRB 060719b 1.5318 1.4 ± 0.4 ± 0.2 0.0 ± 0.3 ± 0.1 ··· 1.7 ± 0.7 ± 0.4 0.5 ± 0.2 ± 0.1
GRB 060729b 0.5429 1.2 ± 1.0 ± 0.2 − 0.2 ± 0.5 ± 0.1 ··· 1.1 ± 0.4 ± 0.1 ···
GRB 060805A 2.3633 0.7 ± 0.4 ± 0.2 1.4 ± 0.6 ± 0.4 0.2 ± 0.4 ± 0.1 1.1 ± 0.2 ± 0.3 5.0 ± 0.6 ± 1.1 − 0.1 ± 0.5 ± 0.1
GRB 060814b 1.9223 26.3 ± 2.0 ± 3.7 ··· 8.4 ± 1.3 ± 1.3 31 ± 6 ± 5 ···
GRB 060912A 0.9362 7.4 ± 0.5 ± 0.7 10.7 ± 0.5 ± 0.9 1.1 ± 0.3 ± 0.1 3.5 ± 0.6 ± 0.3 12.2 ± 1.2 ± 1.1 ···
GRB 060923B 1.5094 ··· 0.1 ± 0.1 ± 0.1 − 0.7 ± 0.4 ± 0.1 1.0 ± 0.4 ± 0.1 − 0.2 ± 0.2 ± 0.1
GRB 060926 3.2090 0.4 ± 0.2 ± 0.2 0.4 ± 0.3 ± 0.2 0.1 ± 0.1 ± 0.1 2.2 ± 0.4 ± 1.0 4.0 ± 0.6 ± 1.6 ···
GRB 061021 0.3453 0.7 ± 0.1 ± 0.1 0.9 ± 0.1 ± 0.1 0.0 ± 0.1 ± 0.1 0.6 ± 0.1 ± 0.1 1.5 ± 0.2 ± 0.2 0.1 ± 0.1 ± 0.1
GRB 061110Ab 0.7578 0.5 ± 0.4 ± 0.2 0.1 ± 0.1 ± 0.1 0.4 ± 0.1 ± 0.2 1.3 ± 0.1 ± 0.5 0.1 ± 0.3 ± 0.1
GRB 061202 2.2543 1.2 ± 0.6 ± 0.3 1.6 ± 0.6 ± 0.4 ··· 1.3 ± 0.2 ± 0.3 3.4 ± 0.3 ± 0.7 − 0.6 ± 0.4 ± 0.1
GRB 070103 2.6208 ··· ··· ··· 5.3 ± 1.1 ± 1.3 10 ± 3 ± 3 ···
GRB 070110b 2.3523 1.7 ± 0.6 ± 0.4 0.1 ± 0.5 ± 0.1 1.9 ± 0.2 ± 0.4 5.9 ± 0.3 ± 1.2 1.0 ± 0.5 ± 0.3
GRB 070129 2.3384 1.8 ± 0.6 ± 0.4 2.1 ± 0.7 ± 0.4 ··· 2.3 ± 0.4 ± 0.4 6.3 ± 1.1 ± 1.1 0.7 ± 1.4 ± 0.3
GRB 070224b 1.9922 0.9 ± 0.4 ± 0.5 0.3 ± 0.5 ± 0.3 0.5 ± 0.2 ± 0.3 1.0 ± 0.2 ± 0.6 ···
GRB 070306 1.4965 9.1 ± 0.6 ± 0.7 7.7 ± 0.8 ± 0.6 1.9 ± 0.3 ± 0.1 15.5 ± 0.6 ± 1.1 46.0 ± 1.6 ± 3.2 6.4 ± 0.3 ± 0.4
GRB 070318 0.8401 1.0 ± 0.2 ± 0.2 1.8 ± 0.2 ± 0.3 0.3 ± 0.1 ± 0.1 1.5 ± 0.2 ± 0.3 4.8 ± 0.3 ± 0.7 − 0.3 ± 0.5 ± 0.1
GRB 070328 2.0627 0.7 ± 0.4 ± 0.2 0.5 ± 0.4 ± 0.2 0.5 ± 0.3 ± 0.1 0.5 ± 0.2 ± 0.1 2.2 ± 0.4 ± 0.4 ···
GRB 070419Bb 1.9586 1.7 ± 0.4 ± 0.4 ··· 1.0 ± 0.3 ± 0.3 2.2 ± 0.6 ± 0.6 ···
GRB 070521b 2.0865 − 2.0 ± 2.0 ± 0.2 ··· ··· 0.2 ± 0.5 ± 0.2 − 0.2 ± 0.9 ± 0.2
GRB 070802 2.4538 1.3 ± 0.3 ± 0.3 2.1 ± 0.3 ± 0.4 0.3 ± 0.2 ± 0.1 1.9 ± 0.1 ± 0.4 4.7 ± 0.3 ± 0.9 1.2 ± 0.9 ± 0.4
GRB 071021 2.4515 1.3 ± 0.8 ± 0.3 2.1 ± 0.7 ± 0.4 0.3 ± 0.8 ± 0.2 2.2 ± 0.5 ± 0.4 5.0 ± 0.6 ± 0.9 0.2 ± 1.0 ± 0.2
GRB 080207b 2.0856 1.0 ± 1.0 ± 0.4 0.4 ± 0.6 ± 0.2 1.7 ± 0.3 ± 0.4 5.6 ± 0.3 ± 1.0 2.5 ± 0.5 ± 0.5
GRB 080413B 1.1012 0.6 ± 0.1 ± 0.1 0.8 ± 0.1 ± 0.2 0.2 ± 0.1 ± 0.1 ··· 2.8 ± 0.5 ± 0.7 ···
GRB 080602 1.8204 7.9 ± 2.3 ± 1.2 7.7 ± 1.1 ± 1.0 0.0 ± 0.6 ± 0.1 ··· 17.0 ± 2.0 ± 2.2 ···
GRB 080605 1.6408 7.9 ± 0.7 ± 0.8 9.2 ± 1.1 ± 1.0 ··· 10.3 ± 0.8 ± 1.6 29.6 ± 1.5 ± 4.4 4.0 ± 0.4 ± 0.6
GRB 080804b 2.2059 0.9 ± 0.9 ± 0.4 0.7 ± 0.7 ± 0.4 ··· 4.9 ± 0.9 ± 1.6 ···
GRB 080805b 1.5052 2.2 ± 0.6 ± 0.4 ··· ··· 3.5 ± 0.8 ± 0.9 0.8 ± 0.2 ± 0.2
GRB 081109 0.9785 6.4 ± 0.5 ± 0.8 10.8 ± 0.5 ± 1.4 ··· ··· 5.7 ± 0.6 ± 0.8 5.7 ± 0.5 ± 0.8
GRB 081210 2.0631 0.9 ± 0.5 ± 0.3 1.2 ± 0.5 ± 0.3 0.8 ± 0.5 ± 0.2 1.7 ± 0.3 ± 0.4 4.3 ± 0.5 ± 0.9 ···
GRB 081221 2.2590 1.2 ± 1.0 ± 1.1 0.9 ± 1.4 ± 1.0 ··· 1.1 ± 0.4 ± 0.7 3.6 ± 0.9 ± 2.1 1.3 ± 1.0 ± 1.1
GRB 090113 1.7494 7.0 ± 2.9 ± 1.5 7.9 ± 2.9 ± 1.6 0.7 ± 1.5 ± 0.3 ··· ··· ···
GRB 090201 2.1000 4.2 ± 2.3 ± 1.2 5.9 ± 2.7 ± 1.6 1.0 ± 1.6 ± 0.5 3.0 ± 0.9 ± 0.7 9.7 ± 0.7 ± 2.0 − 0.4 ± 1.2 ± 0.2
GRB 090323 3.5832 0.8 ± 0.3 ± 0.2 1.0 ± 0.2 ± 0.2 0.1 ± 0.3 ± 0.1 ··· ··· ···
GRB 090407b 1.4478 1.3 ± 0.2 ± 0.2 0.2 ± 0.1 ± 0.1 0.0 ± 0.3 ± 0.1 1.0 ± 0.4 ± 0.2 1.1 ± 0.2 ± 0.2
GRB 090926B 1.2427 4.8 ± 0.3 ± 0.7 6.2 ± 0.3 ± 0.9 1.1 ± 0.2 ± 0.2 4.4 ± 1.3 ± 0.8 13.8 ± 1.5 ± 2.1 1.3 ± 1.2 ± 0.3
GRB 091018b 0.9710 4.2 ± 0.8 ± 0.4 ··· 1.6 ± 0.5 ± 0.1 4.1 ± 0.9 ± 0.3 1.3 ± 0.5 ± 0.1
GRB 091127 0.4904 3.0 ± 0.5 ± 0.3 4.5 ± 0.5 ± 0.4 0.3 ± 0.4 ± 0.1 2.6 ± 0.2 ± 0.2 8.0 ± 0.4 ± 0.7 0.4 ± 0.3 ± 0.1
GRB 100316Da 0.0592 63 ± 3 92 ± 5 18.1 ± 0.9 83 ± 4 253 ± 13 12.2 ± 0.6
GRB 100418Ac 0.6235 33.6 ± 1.8 ± 3.4 1.4 ± 0.6 ± 0.2 8.9 ± 0.6 ± 0.9 26.3 ± 1.5 ± 2.7 4.1 ± 1.8 ± 0.6
GRB 100424A 2.4656 1.1 ± 0.6 ± 0.4 2.4 ± 0.4 ± 0.7 1.4 ± 0.4 ± 0.4 4.5 ± 0.3 ± 1.1 12.5 ± 0.7 ± 3.1 ···
GRB 100508A 0.5201 9.2 ± 2.2 ± 0.7 11.7 ± 1.8 ± 0.8 3.0 ± 1.3 ± 0.3 2.7 ± 0.7 ± 0.2 ··· 4.7 ± 1.5 ± 0.4
GRB 100606A 1.5545 ··· ··· ··· ··· ··· 0.9 ± 0.3 ± 0.3
GRB 100615A 1.3978 1.4 ± 0.1 ± 0.2 1.8 ± 0.1 ± 0.3 0.4 ± 0.1 ± 0.1 3.0 ± 0.4 ± 0.5 6.5 ± 0.5 ± 1.0 0.6 ± 0.3 ± 0.1
GRB 100621A 0.5426 41 ± 2 ± 2 50 ± 2 ± 3 12.4 ± 1.1 ± 0.7 51 ± 4 ± 3 150 ± 3 ± 8 7.6 ± 11.2 ± 1.0
GRB 100724A 1.2890 0.8 ± 0.1 ± 0.2 1.4 ± 0.1 ± 0.4 0.1 ± 0.1 ± 0.1 ··· 2.3 ± 0.9 ± 0.8 0.3 ± 0.4 ± 0.2
GRB 100728A 1.5670 1.6 ± 0.4 ± 0.8 3.3 ± 0.5 ± 1.5 0.3 ± 0.7 ± 0.4 ··· 3.4 ± 1.6 ± 1.9 ···
GRB 100814A 1.4392 0.9 ± 0.1 ± 0.1 1.4 ± 0.1 ± 0.2 0.7 ± 0.1 ± 0.1 2.0 ± 0.4 ± 0.3 5.5 ± 0.7 ± 0.6 0.3 ± 0.2 ± 0.1
GRB 100816Ab 0.8048 5.2 ± 1.0 ± 0.5 0.5 ± 1.3 ± 0.1 0.3 ± 0.9 ± 0.1 1.5 ± 0.6 ± 0.2 6.6 ± 2.2 ± 1.4
GRB 110808A 1.3490 1.7 ± 0.3 ± 0.3 3.2 ± 0.7 ± 0.5 1.6 ± 0.2 ± 0.3 ··· 14.3 ± 1.0 ± 2.1 − 0.1 ± 0.3 ± 0.1
GRB 110818A 3.3609 2.1 ± 0.4 ± 0.3 2.3 ± 0.3 ± 0.3 0.6 ± 0.2 ± 0.1 3.7 ± 0.5 ± 0.5 11.0 ± 0.9 ± 1.5 ···
GRB 110918Ac 0.9843 17.6 ± 2.7 ± 1.0 2.0 ± 2.7 ± 0.2 2.6 ± 2.2 ± 0.2 7.1 ± 1.9 ± 0.4 14.1 ± 4.0 ± 1.2
GRB 111123A 3.1513 4.0 ± 0.5 ± 0.6 3.2 ± 0.4 ± 0.5 1.8 ± 0.4 ± 0.3 1.3 ± 1.0 ± 0.3 7.9 ± 1.6 ± 1.3 ···
GRB 111129Ab 1.0796 7.7 ± 1.8 ± 0.8 − 0.4 ± 0.5 ± 0.1 ··· 7.7 ± 3.5 ± 0.9 ···
GRB 111209A 0.6770 1.1 ± 0.2 ± 0.2 1.4 ± 0.2 ± 0.2 0.3 ± 0.1 ± 0.1 1.1 ± 0.2 ± 0.1 2.9 ± 0.2 ± 0.3 − 0.2 ± 0.3 ± 0.1
GRB 111211A 0.4786 1.6 ± 0.9 ± 0.2 0.7 ± 0.8 ± 0.1 − 0.4 ± 0.8 ± 0.1 0.7 ± 0.4 ± 0.1 2.7 ± 0.7 ± 0.2 ···
GRB 111228A 0.7164 0.7 ± 0.3 ± 0.1 1.2 ± 0.3 ± 0.1 − 0.1 ± 0.2 ± 0.1 0.8 ± 0.2 ± 0.1 1.2 ± 0.3 ± 0.1 ···
GRB 120118B 2.9428 2.5 ± 0.6 ± 0.4 4.2 ± 1.5 ± 0.8 2.4 ± 0.3 ± 0.4 ··· 32 ± 3 ± 5 ···
GRB 120119Ab 1.7291 1.6 ± 2.6 ± 0.5 0.8 ± 0.8 ± 0.3 ··· ··· 2.6 ± 0.3 ± 0.5
GRB 120422A 0.2826 28.7 ± 0.8 ± 1.1 42.8 ± 0.9 ± 1.6 2.7 ± 0.3 ± 0.1 8.6 ± 0.5 ± 0.3 30.6 ± 1.2 ± 1.1 8.4 ± 0.3 ± 0.3
GRB 120624B 2.1974 4.7 ± 0.9 ± 1.6 3.8 ± 0.8 ± 1.3 1.1 ± 0.8 ± 0.5 6.0 ± 1.5 ± 2.1 16.7 ± 1.3 ± 5.1 2.7 ± 1.4 ± 1.2
GRB 120714B 0.3985 4.1 ± 0.4 ± 0.3 5.7 ± 0.3 ± 0.4 1.1 ± 0.2 ± 0.1 2.9 ± 0.3 ± 0.2 7.7 ± 0.5 ± 0.5 0.6 ± 0.2 ± 0.1
GRB 120722A 0.9590 10.3 ± 0.4 ± 1.1 11.7 ± 0.4 ± 1.2 1.2 ± 0.2 ± 0.2 7.1 ± 0.8 ± 0.8 27.2 ± 1.3 ± 2.9 4.1 ± 0.8 ± 0.5
GRB 120815Ab 2.3587 0.5 ± 0.4 ± 0.2 0.3 ± 0.2 ± 0.1 0.6 ± 0.1 ± 0.2 1.5 ± 0.1 ± 0.4 0.1 ± 0.2 ± 0.1
GRB 121024A 2.3012 6.7 ± 0.7 ± 0.6 7.2 ± 0.7 ± 0.6 ··· 12.2 ± 0.6 ± 1.0 31.9 ± 1.3 ± 2.6 1.8 ± 0.9 ± 0.2
GRB 121027A 1.7732 4.0 ± 3.2 ± 0.6 4.2 ± 2.1 ± 0.5 ··· 3.5 ± 1.0 ± 0.4 14.2 ± 3.1 ± 1.5 ···
GRB 121201A 3.3830 1.0 ± 0.4 ± 0.1 1.7 ± 0.7 ± 0.2 1.6 ± 0.7 ± 0.2 ··· ··· ···
GRB 130131B 2.5393 0.7 ± 0.3 ± 0.2 0.6 ± 0.4 ± 0.2 ··· 0.7 ± 0.3 ± 0.2 1.5 ± 0.2 ± 0.3 ···
GRB 130427A 0.3401 9.1 ± 1.7 ± 0.7 11.1 ± 1.5 ± 0.9 0.0 ± 1.1 ± 0.1 0.9 ± 0.8 ± 0.1 6.5 ± 1.0 ± 0.5 1.5 ± 0.6 ± 0.2
GRB 130701Ab 1.1548 1.3 ± 1.8 ± 0.2 0.4 ± 0.9 ± 0.1 0.8 ± 4.7 ± 0.3 11.0 ± 6.6 ± 1.1 ···
GRB 130925Ac 0.3483 25.8 ± 0.8 ± 1.6 1.2 ± 0.7 ± 0.1 5.6 ± 0.8 ± 0.3 18.7 ± 0.7 ± 0.9 11.7 ± 0.5 ± 0.6
GRB 131103Ac 0.5960 40.4 ± 4.0 ± 5.9 5.5 ± 3.6 ± 1.2 22.8 ± 1.6 ± 3.3 66 ± 4 ± 11 2.6 ± 1.2 ± 0.5
GRB 131105Ab 1.6854 7.5 ± 1.6 ± 1.0 1.1 ± 0.8 ± 0.4 0.8 ± 0.8 ± 0.3 3.2 ± 1.6 ± 1.0 1.4 ± 0.5 ± 0.4
GRB 131231A 0.6427 2.9 ± 0.6 ± 0.3 4.4 ± 0.6 ± 0.4 1.0 ± 0.4 ± 0.1 6.6 ± 0.5 ± 0.6 17.0 ± 0.9 ± 1.4 1.5 ± 0.5 ± 0.2
GRB 140213A 1.2079 ··· ··· ··· 1.0 ± 0.8 ± 0.2 0.8 ± 0.5 ± 0.1 ···
GRB 140301A 1.4155 3.3 ± 0.5 ± 0.3 3.9 ± 0.3 ± 0.3 ··· 1.2 ± 0.8 ± 0.2 4.1 ± 0.7 ± 0.4 10.9 ± 0.5 ± 0.9
GRB 140430Ab 1.6019 1.8 ± 1.2 ± 0.2 ··· ··· 10.7 ± 1.8 ± 1.0 1.3 ± 0.6 ± 0.2
GRB 140506A 0.8893 0.6 ± 0.1 ± 0.1 0.7 ± 0.1 ± 0.1 0.1 ± 0.1 ± 0.1 ··· ··· − 0.0 ± 0.2 ± 0.1

Notes. Measurements are in units of 10-17 erg cm-2 s-1, and are corrected for the Galactic foreground reddening. A correction for slit-loss based on broad-band photometry has been applied to the measurements as described in the text. These values thus represent host-integrated measurements except for GRB 100316D (see below). Line fluxes are not corrected for host-intrinsic extinction. The first error represents the statistical error due to photon statistics and line-flux measurement. The second error is the systematic error in the absolute flux calibration due to slit-loss and scaling to photometry. Redshifts are given in a heliocentric reference frame. No data means that either the wavelength range of the respective line is not covered, all data in that wavelength range have been excluded from the automated fitting procedure, or no meaningful constraints could be obtained for the given line.

(a)

GRB 100316D has the lowest redshift in the sample (z = 0.0592). The fraction of the host that is covered by the slit is too small to derive representative host-integrated measurements. These values are thus as derived from the observed spectrum and not scaled by photometry. No systematic error on the line fluxes is given in this case.

(b)

In these cases, we can not constrain the individual components of the [O ii] doublet well, either because of telluric absorption, skylines or low signal-to-noise level. We constrain the ratio between the two components to be between 2/3 and 3/2, and provide the measurement for the combined fit of [O ii](λ3726) and [O ii](λ3729).

(c)

These galaxies have non-trivial velocity structure. We are not able to uniquely disentangle the individual components of the [O ii] doublet, so we provide the total [O ii] flux instead.

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