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Table 4

Physical properties of GRB hosts.

GRB hosta Redshift E B − V SF-tracer SFR b σ Z
(mag) (M⊙ yr-1) (km s-1) 12 + log (O/H)
GRB 050416A 0.6542 Hα 47 ± 4
GRB 050525A 0.6063 Hα 26 ± 5 ···
GRB 050714B 2.4383 Hα 35 ± 16 ···
GRB 050819A 2.5042 Hβ 50 ± 6 ···
GRB 050824 0.8277 Hα 48 ± 5
GRB 050915A 2.5275 Hβ 87 ± 10 ···
GRB 051001 2.4295 Hα 67 ± 8 ···
GRB 051016B 0.9358 Hα 58 ± 4
GRB 051022A 0.8061 Hα 88 ± 5
GRB 051117B 0.4805 Hα 85 ± 11
GRB 060204B 2.3393 Hα 85 ± 8 ···
GRB 060306 1.5597 Hα 60 ± 14 ···
GRB 060604 2.1355 Hα 68 ± 13
GRB 060707 3.4246 ··· [O ii] ··· ···
GRB 060719 1.5318 Hα 42 ± 5
GRB 060729 0.5429 Hα 66 ± 16 ···
GRB 060805A 2.3633 Hα 71 ± 7 ···
GRB 060814 1.9223 Hα 132 ± 11 ···
GRB 060912A 0.9362 Hα 62 ± 5
GRB 060923B 1.5094 ··· Hα 46 ± 15 ···
GRB 060926 3.2090 ··· [O iii] 60 ± 8 ···
GRB 061021 0.3453 Hα 16.1 ± 4.8 ···
GRB 061110A 0.7578 ··· Hβ 31 ± 4 ···
GRB 061202 2.2543 Hα 64 ± 7 ···
GRB 070103 2.6208 Hβ 124 ± 30 ···
GRB 070110 2.3523 Hα 24 ± 4 ···
GRB 070129 2.3384 Hα 76 ± 11 ···
GRB 070224 1.9922 ··· [O iii] 37 ± 9 ···
GRB 070306 1.4965 Hα 121 ± 55
GRB 070318 0.8401 Hα 53 ± 5 ···
GRB 070328 2.0627 Hβ 93 ± 14 ···
GRB 070419B 1.9586 Hα 86 ± 10 ···
GRB 070521 2.0865 ··· Hα 249 ± 108 ···
GRB 070802 2.4538 Hα 57 ± 5 ···
GRB 071021 2.4515 Hα 100 ± 17 ···
GRB 080207 2.0856 Hα 136 ± 18
GRB 080413B 1.1012 Hα 39 ± 5
GRB 080602 1.8204 Hα 91 ± 13 ···
GRB 080605 1.6408 Hα 80 ± 6
GRB 080804 2.2059 Hα 50 ± 9 ···
GRB 080805 1.5052 Hα 54 ± 12
GRB 081109 0.9785 Hα 108 ± 6
GRB 081210 2.0631 Hβ 118 ± 12 ···
GRB 081221 2.2590 Hα 93 ± 12 ···
GRB 090113 1.7494 Hα 70 ± 9 ···
GRB 090201 2.1000 Hα 171 ± 12 ···
GRB 090323 3.5832 ··· [O ii] 60 ± 13 ···
GRB 090407 1.4478 Hα 109 ± 8
GRB 090926B 1.2427 Hα 65 ± 4
GRB 091018 0.9710 Hα 57 ± 10
GRB 091127 0.4904 Hα 30 ± 5
GRB 100418A 0.6235 Hα 56 ± 4
GRB 100424A 2.4656 Hβ 87 ± 5
GRB 100508A 0.5201 Hα 80 ± 11
GRB 100606A 1.5545 Hα 107 ± 36
GRB 100615A 1.3978 Hα 45 ± 5
GRB 100621A 0.5426 Hα 82 ± 4
GRB 100724A 1.2890 Hα 58 ± 7 ···
GRB 100728A 1.5670 Hα 57 ± 8 ···
GRB 100814A 1.4392 Hα 31 ± 5 ···
GRB 100816A 0.8048 Hα 111 ± 30
GRB 110808A 1.3490 Hα 40 ± 4
GRB 110818A 3.3609 ··· Hβ 89 ± 8
GRB 110918A 0.9843 Hα 126 ± 18
GRB 111123A 3.1513 ··· [O ii] 135 ± 21
GRB 111129A 1.0796 ··· [O ii] 117 ± 35 ···
GRB 111209A 0.6770 Hα 35 ± 5
GRB 111211A 0.4786 Hα 38 ± 8 ···
GRB 111228A 0.7164 ··· Hβ 19.7 ± 5.5 ···
GRB 120118B 2.9428 Hβ 193 ± 8
GRB 120119A 1.7291 Hα 104 ± 17
GRB 120422A 0.2826 Hα 25 ± 4
GRB 120624B 2.1974 Hα 77 ± 6
GRB 120714B 0.3985 Hα 34 ± 4
GRB 120722A 0.9590 Hα 56 ± 4
GRB 120815A 2.3587 Hα 28 ± 5 ···
GRB 121024A 2.3012 Hα 88 ± 4
GRB 121027A 1.7732 ··· [O iii] 119 ± 75 ···
GRB 121201A 3.3830 ··· [O ii] 86 ± 17 ···
GRB 130131B 2.5393 ··· [O iii] 73 ± 29 ···
GRB 130427A 0.3401 Hα 40 ± 5
GRB 130701A 1.1548 ··· [O ii] 82 ± 42 ···
GRB 130925A 0.3483 Hα 49 ± 5
GRB 131103A 0.5960 Hα 87 ± 7
GRB 131105A 1.6854 Hα 52 ± 11
GRB 131231A 0.6427 Hα 33 ± 4
GRB 140213A 1.2079 Hα 34 ± 14 ···
GRB 140301A 1.4155 Hα 117 ± 6
GRB 140430A 1.6019 ··· Hα 40 ± 7
GRB 140506A 0.8893 ··· Hα 61 ± 9 ···

Notes.

(a)

The physical parameters presented here are integrated and thus averaged over the entire galaxy. We do not perform a resolved analysis (neither spatially, nor in velocity space). In some cases (e.g., GRB 120422A, Schulze et al. 2014), a spatially resolved analysis leads to somewhat different results and interpretation of the galaxy properties.

(b)

The quoted error on SFR is logarithmic because it contains the error in the dust correction. The derived SFR also has a lower limit because of the physical condition that AV> 0 mag. This lower limit is given by SFRmin = 4.8 × FHα,42.

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