Table 3
Voigt-profile fitting (best fits shown in Fig. 8) of metal ion transitions in the DLA using FITLYMAN.
| λobs | E Wobs | σEW | E Wrest | ID | zabs | log N | bturb | [X/H] | |
| Å | Å | Å | Å | cm-2 | km s-1 | ||||
|
|
|||||||||
| 3634.960 | ... | ... | ... | N v (1238) | 1.93421 | <12.71 | ... | ||
| 3646.650 | ... | ... | ... | N v (1242) | 1.93421 | <12.71 | ... | ||
| 3519.770 | 0.070 | 0.030 | ... | N i (1199) | 1.93424 | 12.95 ± 0.12 | ... | ||
| 3820.900 | 0.681 | 0.029 | 0.232 | O i (1302) | 1.93426 | >14.97 | 20.1 ± 2.1 | [O/H] > −2.06 | |
| 3915.800 | 0.724 | 0.037 | 0.247 | C ii (1334) | 1.93421 | >14.46 | 18.8 ± 0.2 | [C/H] > −2.31 | |
| 3919.150 | 0.050 | 0.015 | 0.017 | C ii* (1335.7) | 1.93414 | 12.94 ± 0.12 | ... | ||
| 4542.600 | 0.928 | 0.040 | 0.316 | C iv (1548) | 1.93413 | >14.56 | 18.9 ± 0.4 | ||
| 4550.155 | 0.813 | 0.035 | 0.277 | C iv (1550) | 1.93413 | >14.56 | 18.9 ± 0.4 | ||
| 3492.924 | 0.790 | 0.023 | ... | Si ii (1190) | 1.93421 | ...a | ... | ||
| 3501.357 | 0.362 | 0.014 | 0.123 | Si ii (1193) | 1.93421 | 13.92 ± 0.03 | 18.6 ± 0.4 | ||
| 3698.343 | 0.767 | 0.034 | 0.261 | Si ii (1260) | 1.93421 | 13.92 ± 0.03 | 18.6 ± 0.4 | ||
| 3827.300 | 0.265 | 0.030 | 0.100 | Si ii (1304) | 1.93421 | 13.92 ± 0.03 | 18.6 ± 0.4 | ||
| 4479.678 | 0.459 | 0.026 | 0.156 | Si ii (1526) | 1.93421 | 13.92 ± 0.03 | 18.6 ± 0.4 | [Si/H] = −1.93 ± 0.04 | |
| 5305.090 | ... | ... | ... | Si ii (1808) | 1.93421 | <14.46 | ... | ||
| 3540.130 | 0.804 | 0.030 | 0.270 | Si iii (1206) | 1.93421 | >13.85 | 18.8 ± 0.3 | ||
| 4089.480 | 0.640 | 0.065 | 0.218 | Si iv (1393) | 1.93415 | >13.75 | 19.2 ± 0.7 | ||
| 4115.933 | 0.517 | 0.035 | 0.180 | Si iv (1402) | 1.93415 | >13.75 | 19.2 ± 0.7 | ||
| 3359.492 | 0.103 | 0.024 | 0.035 | Fe ii (1144) | 1.93421 | 13.60 ± 0.02 | 18.8 ± 0.3 | [Fe/H] = −2.24 ± 0.03 | |
| 4719.540 | 0.144 | 0.035 | 0.049 | Fe ii (1608) | 1.93421 | 13.60 ± 0.02 | 18.8 ± 0.3 | ||
| 4727.600 | ... | ... | ... | Fe ii (1611) | 1.93421 | <14.67 | ... | ||
| 6967.170 | 0.138 | 0.010 | 0.047 | Fe ii (2374) | 1.93421 | 13.60 ± 0.02 | 18.8 ± 0.3 | ||
| 6991.530 | 0.883 | 0.010 | 0.301 | Fe ii (2382) | 1.93421 | 13.60 ± 0.02 | 18.8 ± 0.3 | ||
| 7589.770 | 0.410 | 0.013 | 0.140 | Fe ii (2586) | 1.93421 | 13.60 ± 0.02 | 18.8 ± 0.3 | ||
| 4902.464 | 0.321 | 0.041 | 0.110 | Al ii (1670) | 1.93423 | 12.46 ± 0.02 | 18.8 ± 0.2 | [Al/H] = −2.33 ± 0.03 | |
| 5442.160 | 0.09 | 0.023 | 0.030 | Al iii (1854) | 1.93423 | 12.15 ± 0.07 | 18.8 ± 0.2 | ||
| 5465.850 | 0.060 | 0.030 | 0.020 | Al iii (1862) | 1.93423 | 12.15 ± 0.07 | 18.8 ± 0.2 | ||
| 8205.080 | 1.611 | 0.010 | 0.550 | Mg ii (2796) | 1.93421 | >13.79 | 18.8 ± 0.3 | [Mg/H] > −2.15 | |
| 8226.140 | 1.380 | 0.011 | 0.470 | Mg ii (2803) | 1.93421 | >13.79 | 18.8 ± 0.3 | ||
| 8371.210 | 0.058 | 0.021 | 0.020 | Mg i (2852) | 1.93421 | 11.19 ± 0.11 | ... | ||
Notes. Ionic column densities were used to derive individual element abundances in the neutral gas phase via comparison to the solar neighbourhood (Asplund et al. 2009). Multiplets were fitted with same column densities and turbulent broadening parameter values. The Si ii λ1808, Fe ii λ1611 and N v lines are not detected and for those we provide 3σ column density upper limits (see text).
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