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Table 1.

GRB line-of-sight metal abundances and the H I, O I* λ1304 and O I** λ1306 column densities.

GRB z log NHI (cm−2) log(Z/Z) log (cm−2) log (cm−2) log β[OI]−63 μm (M/L) log β[OI]−145 μm (M/L)
090809A 2.7373 21.48 ± 0.07 −0.46 ± 0.15 15.28 ± 0.68 15.28 ± 0.68 0.26 ± 0.69 2.22 ± 0.50
090926A 2.1069 21.58 ± 0.01 −1.72 ± 0.05 14.77 ± 0.06 14.77 ± 0.06 0.87 ± 0.06 2.19 ± 0.05
100219A 4.6676 21.28 ± 0.02 −1.16 ± 0.11 13.71 ± 0.53 13.71 ± 0.53 1.63 ± 0.53 3.12 ± 0.89
111008A 4.9910 22.39 ± 0.01 −1.79 ± 0.10 14.25 ± 0.78 14.25 ± 0.78 2.21 ± 0.78 2.88 ± 0.39
120815A 2.3582 22.09 ± 0.01 −1.23 ± 0.03 15.17 ± 0.42 15.17 ± 0.42 0.98 ± 0.42 2.65 ± 0.12
120909A 3.9290 21.82 ± 0.02 −0.29 ± 0.10 15.21 ± 0.56 15.21 ± 0.56 0.67 ± 0.56 2.16 ± 0.14
130408A 3.7579 21.90 ± 0.01 −1.46 ± 0.05 14.38 ± 0.38 14.38 ± 0.38 1.58 ± 0.38 1.56 ± 0.24
140311A 4.9550 22.30 ± 0.02 −2.00 ± 0.11 14.40 ± 0.55 14.40 ± 0.55 1.96 ± 0.55 3.59 ± 0.71
150403A 2.0571 21.73 ± 0.02 −0.92 ± 0.05 15.49 ± 0.28 15.49 ± 0.28 0.30 ± 0.28 2.03 ± 0.13
151021A 2.3297 22.14 ± 0.03 −0.97 ± 0.07 14.50 ± 0.41 14.50 ± 0.41 1.70 ± 0.41 2.63 ± 0.23
151027B 4.0650 20.54 ± 0.07 −0.59 ± 0.27 14.99 ± 0.30 14.99 ± 0.30 −0.39 ± 0.31 1.63 ± 0.31
160203A 3.5187 21.74 ± 0.02 −0.92 ± 0.04 14.50 ± 0.55 14.50 ± 0.55 1.30 ± 0.55 2.96 ± 0.58
161023A 2.7100 20.95 ± 0.01 −1.05 ± 0.04 14.92 ± 0.10 14.92 ± 0.10 0.09 ± 0.10 1.76 ± 0.04
170202A 3.6456 21.53 ± 0.04 −1.02 ± 0.13 14.43 ± 0.12 14.43 ± 0.12 1.16 ± 0.13 3.03 ± 0.32
181020A 2.9379 22.24 ± 0.03 −1.20 ± 0.08 15.38 ± 0.27 15.38 ± 0.27 0.92 ± 0.27 3.18 ± 0.30
190106A 1.8599 21.00 ± 0.04 −0.40 ± 0.10 15.40 ± 0.12 15.40 ± 0.12 −0.34 ± 0.13 2.67 ± 0.90
190114A 3.3764 22.19 ± 0.05 −1.17 ± 0.06 15.32 ± 0.48 15.32 ± 0.48 0.93 ± 0.48 2.34 ± 0.34
191011A 1.7204 21.65 ± 0.08 −0.63 ± 0.07 14.40 ± 0.39 14.40 ± 0.39 1.31 ± 0.39 2.86 ± 0.53
210905A 6.3118 21.00 ± 0.02 −1.24 ± 0.10 14.73 ± 0.52 14.73 ± 0.52 0.33 ± 0.52 2.27 ± 0.38

Notes. The H I column densities and dust-corrected gas-phase metallicities are partly from Bolmer et al. (2019) and partly from Heintz et al. (in prep.). The O I* λ1304 and O I** λ1306 column densities are derived in this work. The last two columns, β[OI]−63 μm and β[OI]−145 μm, denote the absorption-derived conversion factors per unit column for each GRB.

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