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Table 2.
Host absorption lines identified in the first X-shooter spectrum, with their measured equivalent widths (observer frame) and column densities.
| Observed λ | Feature | EW | log(N/cm−2) |
|---|---|---|---|
| (Å) | (Å) | ||
| 4530.09 | Ca II 3934.78 | 1.58 ± 0.1 | > 15.5 |
| 4570.44 | Ca II 3969.59 | 1.35 ± 0.09 | |
| 4867.40 | Ca I 4227.92 | 0.36 ± 0.06 | 12.19 ± 0.08 |
| 6782.87 | Na I 5891.58 | 0.29 ± 0.01 | 12.21 ± 0.01 |
| 6789.71 | Na I 5897.56 | 0.15 ± 0.01 | |
| 12 470.76 | He I* 10830 | 1.025 ± 0.015 | 12.29 ± 0.01 (a) |
Notes. (a) Best-fit column density with 
and b = 40.9 ± 1.3 km s−1.
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