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Table 1.

Overview of the absorption-derived GRB host galaxy ISM properties.

GRB zGRB AV (SED) log NHI [X/H] X [Zn/Fe] [M/H]tot Telescope/ Ref.
(mag) (cm−2) Instrument
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
000926 2.0380 0.38 ± 0.05 21.30 ± 0.20 −0.11 ± 0.21 Zn 1.06 ± 0.18 0.20 ± 0.28 Keck/ESI (1,2)
030226 1.9870 20.50 ± 0.30 −0.94 ± 0.30 Si −0.18 ± 0.12 −1.07 ± 0.31 Keck/ESI (3,4)
050730 3.9690 0.12 ± 0.02 22.10 ± 0.10 −2.18 ± 0.11 S 0.08 ± 0.05 −2.31 ± 0.18 VLT/UVES (2,5,6)
050820A 2.6150 0.27 ± 0.04 21.05 ± 0.10 −0.39 ± 0.10 Zn 0.83 ± 0.05 −0.49 ± 0.10 VLT/UVES+HIRES (2,4,5,6)
050922C 2.1990 0.09 ± 0.03 21.55 ± 0.10 −2.09 ± 0.12 Si 0.18 ± 0.46 −1.92 ± 0.26 VLT/UVES (5,7)
071031 2.6920 < 0.07 22.15 ± 0.05 −1.76 ± 0.05 Zn 0.04 ± 0.03 −1.75 ± 0.09 VLT/UVES (5)
080413A 2.4330 < 0.59 21.85 ± 0.15 −1.63 ± 0.16 Zn 0.13 ± 0.07 −1.60 ± 0.18 VLT/UVES (5)
081008 1.9685 < 0.08 21.11 ± 0.10 −0.52 ± 0.11 Zn 0.55 ± 0.04 −0.51 ± 0.17 VLT/UVES (6,8)
090809A 2.7373 0.11 ± 0.04 21.48 ± 0.07 −0.86 ± 0.13 Zn 0.75 ± 0.21 −0.46 ± 0.15 VLT/X-shooter (9)
090926A 2.1069 < 0.03 21.58 ± 0.01 −1.97 ± 0.11 Zn 0.84 ± 0.05 −1.72 ± 0.05 VLT/X−shooter (9,10)
100219A 4.6676 0.15 ± 0.05 21.28 ± 0.02 −1.24 ± 0.05 S 0.12 ± 0.30 −1.16 ± 0.11 VLT/X-shooter (9,11)
111008A 4.9910 0.13 ± 0.05 22.39 ± 0.01 −1.48 ± 0.31 Zn 0.22 ± 0.10 −1.79 ± 0.10 VLT/X-shooter (9,12)
111107A 2.8930 < 0.15 21.10 ± 0.04 −0.74 ± 0.2 Si 0.70 ± 0.55 −0.28 ± 0.45 VLT/X-shooter (9)
120119A 1.7285 1.06 ± 0.02 22.44 ± 0.12 −1.03 ± 0.25 Zn 0.93 ± 0.24 −0.79 ± 0.42 VLT/X-shooter (6)
120327A 2.8143 0.05 ± 0.02 22.07 ± 0.01 −1.49 ± 0.04 Zn 0.34 ± 0.03 −1.34 ± 0.02 VLT/X-shooter (9,13)
120716A 2.4874 0.30 ± 0.15 21.73 ± 0.03 −0.71 ± 0.06 Zn 0.60 ± 0.15 −0.57 ± 0.08 VLT/X-shooter (9)
120815A 2.3582 0.19 ± 0.04 22.09 ± 0.01 −1.45 ± 0.03 Zn 0.95 ± 0.04 −1.23 ± 0.03 VLT/X-shooter (9,14)
120909A 3.9290 0.16 ± 0.04 21.82 ± 0.02 −1.06 ± 0.12 S 1.15 ± 0.09 −0.29 ± 0.10 VLT/X-shooter (9)
121024A 2.3005 0.26 ± 0.07 21.78 ± 0.02 −0.76 ± 0.06 Zn 0.73 ± 0.07 −0.68 ± 0.07 VLT/X-shooter (9,15)
130408A 3.7579 0.12 ± 0.03 21.90 ± 0.01 −1.48 ± 0.07 Zn 0.29 ± 0.07 −1.46 ± 0.05 VLT/X-shooter (9)
130606A 5.9127 < 0.03 19.88 ± 0.01 −1.83 ± 0.10 Si 0.49 ± 0.10 −1.58 ± 0.08 VLT/X-shooter (9,16)
140311A 4.9550 0.07 ± 0.03 22.30 ± 0.02 −1.65 ± 0.14 Zn 0.23 ± 0.11 −2.00 ± 0.11 VLT/X-shooter (9)
141028A 2.3333 0.13 ± 0.09 20.39 ± 0.03 −1.64 ± 0.13 Si −0.04 ± 0.26 −1.62 ± 0.28 VLT/X-shooter (9)
141109A 2.9940 0.16 ± 0.04 22.18 ± 0.02 −1.63 ± 0.06 Zn 0.61 ± 0.05 −1.37 ± 0.05 VLT/X-shooter (9)
150403A 2.0571 0.12 ± 0.02 21.73 ± 0.02 −1.04 ± 0.04 Zn 0.47 ± 0.05 −0.92 ± 0.05 VLT/X-shooter (9)
151021A 2.3297 0.20 ± 0.03 22.14 ± 0.03 −0.98 ± 0.07 Zn 0.69 ± 0.07 −0.97 ± 0.07 VLT/X-shooter (9)
151027B 4.0650 0.10 ± 0.05 20.54 ± 0.07 −0.76 ± 0.17 S 0.49 ± 0.64 −0.59 ± 0.27 VLT/X-shooter (9)
160203A 3.5187 < 0.10 21.74 ± 0.02 −1.31 ± 0.04 S 0.37 ± 0.18 −0.92 ± 0.04 VLT/X-shooter (9, 17)
161023A 2.7100 0.09 ± 0.03 20.95 ± 0.01 −1.23 ± 0.03 S 0.44 ± 0.04 −1.05 ± 0.04 VLT/X-shooter (9,18)
170202A 3.6456 0.08 ± 0.03 21.53 ± 0.04 −1.28 ± 0.09 S 0.76 ± 0.23 −1.02 ± 0.13 VLT/X-shooter (9)
181020A 2.9379 0.29 ± 0.02 22.24 ± 0.03 −1.57 ± 0.11 Zn 0.76 ± 0.14 −1.20 ± 0.08 VLT/X-shooter (19,20)
190106A 1.8599 0.27 ± 0.03 21.00 ± 0.04 −0.33 ± 0.10 Zn 1.13 ± 0.10 −0.40 ± 0.10 VLT/X-shooter (20)
190114A 3.3764 0.34 ± 0.01 22.19 ± 0.05 −1.44 ± 0.24 S 1.06 ± 0.08 −1.17 ± 0.06 VLT/X-shooter (19,20)
190919B 3.2241 < 0.03 21.49 ± 0.03 −1.40 ± 0.16 S 0.33 ± 0.33 −1.25 ± 0.15 VLT/X-shooter (20)
191011A 1.7204 0.43 ± 0.03 21.65 ± 0.08 −0.95 ± 0.11 Zn 0.33 ± 0.09 −0.63 ± 0.08 VLT/X-shooter (20)
210905A 6.3118 < 0.02 21.10 ± 0.10 −1.71 ± 0.11 Si 0.33 ± 0.09 −1.72 ± 0.13 VLT/X-shooter (21)

Notes. This table is composed mainly of GRB afterglow measurements from the literature, in addition to the three new bursts analyzed here: GRBs 190106A, 190919B, and 191011A. Column (1): GRB names. Column (2): spectroscopic redshift of the absorption system. Column (3): visual extinction derived from the SED. Upper limits are reported at 1σ. Column (4): H I column density derived from the Lyman-α absorption feature. Column (5): Metallicity of the element X. Column (6): element X used for the metallicity and depletion measurements. Column (7): Zinc-over-iron depletion level. Column (8): dust-corrected metallicity. Column (9): Telescope and instrument with which the GRB afterglows were observed. Column (10): references for the first afterglow spectra presentations and subsequent measurements adopted in this work.

References. (1) Savaglio et al. (2003); (2) Zafar & Møller (2019); (3) Shin et al. (2006); (4) Prochaska et al. (2007); (5) Ledoux et al. (2009); (6) Wiseman et al. (2017), (7) Piranomonte et al. (2008); (8) D’Elia et al. (2014); (9) Bolmer et al. (2019); (10) D’Elia et al. (2010); (11) Thöne et al. (2013); (12) Sparre et al. (2014); (13) D’Elia et al. (2014); (14) Krühler et al. (2013); (15) Friis et al. (2015); (16) Hartoog et al. (2015); (17) Pugliese et al. (2023); (18) de Ugarte Postigo et al. (2018); (19) Heintz et al. (2019a); (20) this work; (21) Saccardi et al. (2023).

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