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Table 3.

Components and column densities (N) with their corresponding b-parameters in the GRB system.

Component I
Component II
Component III
Component IV
Total
Ion Transitions vb log(N/cm−2) vb log(N/cm−2) vb log(N/cm−2) vb log(N/cm−2) log(N/cm−2)
Å (km s−1) (km s−1) (km s−1) (km s−1)
HI Lyα to Ly9 20.97 ± 0.01
S II 1250, 1253, (1259) 0 22 14.69 ± 0.02 –76 15 14.33 ± 0.04 –188 28 14.20 ± 0.05 14.94 ± 0.02
Si II 1260, 1304, 1526, 1808 0 22 14.54 ± 0.02 –76 15 14.77 ± 0.03 –188 28 13.97 ± 0.02 15.04 ± 0.02
O I 1302 0 15 < 17.2 –76 15 < 16.0 –188 30 14.58 ± 0.01 < 17.2
C II 1334 0 22 15.30 ± 0.10 –76 15 15.80 ± 0.10 –142 30 13.78 ± 0.02 –188 28 14.56 ± 0.01 15.94 ± 0.04
Fe II 1608, 2260, 2344, 2374 0 22 14.43 ± 0.02 –76 15 14.18 ± 0.02 –188 28 13.56 ± 0.06 14.66 ± 0.01
(2382, 2586, 2600)
Al II 1670 0 22 13.23 ± 0.01 –76 15 14.03 ± 0.05 –142 30 12.99 ± 0.01 –188 28 12.81 ± 0.02 14.14 ± 0.02
Zn II 2026 0 22 12.01 ± 0.09 –76 15 11.84 ± 0.12 –188 30 11.96 ± 0.10 12.42 ± 0.06
Mg II 2796, 2803 0 21 13.80 ± 0.1 –95 43 14.85 ± 0.27 –188 32 13.86 ± 0.04 15.08 ± 0.20
Mg I 2026, 2852 0 50 12.24 ± 0.06 –95 25 12.17 ± 0.06 –188 32 12.42 ± 0.03 12.76 ± 0.03

Fe II1s 2333, 2612, 2626 0 13 13.32 ± 0.02 –76 25 13.26 ± 0.03 –188 20 12.92 ± 0.04 13.68 ± 0.08
Fe II3s 2338, 2359, (2631) 0 13 12.63 ± 0.08 –76 25 12.80 ± 0.06 –188 20 12.49 ± 0.12 13.13 ± 0.05
Fe II4s 2345, 2629 0 13 12.90 ± 0.03 –76 25 12.48 ± 0.10 13.03 ± 0.02
Fe II 5s 1637, 1702 0 13 13.19 ± 0.04 –76 25 13.13±0.06 –188 20 12.89 ± 0.09 13.56 ± 0.03
Ni II2s 2217, 2316 0 13 13.17 ± 0.01 –76 25 13.03 ± 0.02 –188 20 12.59 ± 0.04 13.46 ± 0.01
Si II* 1309, 1533 0 27 14.08 ± 0.01 –76 35 14.04 ± 0.01 –142 30 13.22 ± 0.05 –188 38 13.95 ± 0.01 14.50 ± 0.01
C II* 1335.6, 1335.7 0 27 13.87 ± 0.01 –76 35 14.38 ± 0.01 –188 38 14.48 ± 0.01 14.79 ± 0.01
O I* 1304 0 33 14.24 ± 0.01 –63 27 14.09 ± 0.02 –176 30 14.50 ± 0.01 14.79 ± 0.01
O I** 1306 0 50 14.52 ± 0.06 –63 15 14.40 ± 0.06 –102 16 14.53 ± 0.03 –176 30 14.46 ± 0.03 15.23 ± 0.04
51 33 14.70 ± 0.04

C IV 1548, 1550 +6 29 13.51 ± 0.03 –83 43 13.19 ± 0.27 –114 27 15.42 ± 0.08 –188 28 13.62 ± 0.03 15.43 ± 0.07
Si IV 1402 +6 29 13.17 ± 0.02 –83 43 13.65 ± 0.02 –114 27 14.44 ± 0.02 –188 28 13.33 ± 0.02 14.55 ± 0.01
N V 1238, 1242 –83 43 13.47 ± 0.03 –114 27 13.54 ± 0.03 –188 28 13.08 ± 0.05 13.88 ± 0.02
S IV 1062 –83 43 14.42 ± 0.02 –114 27 14.07 ± 0.05 –188 28 13.68 ± 0.06 14.63 ± 0.02
S VI 933, 944 –83 43 13.52 ± 0.05 –114 27 13.97 ± 0.03 –188 28 13.16 ± 0.09 14.15 ± 0.03
O VI 1031, (1037) +6 29 13.77 ± 0.03 –83 43 14.22 ± 0.02 –114 27 14.33 ± 0.02 –188 28 13.94 ± 0.02 14.72 ± 0.15
P V 1117, 1128 –28 25 13.54 ± 0.01 –103 25 13.13 ± 0.02 13.68 ± 0.01

Notes. Their velocity (v) is defined with respect to the highest redshift component, which we define as having v = 0 km s−1. Transitions in brackets are detected but were not used for the fit due to either blending with other lines or large errors due to sky emission lines.

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