Table 2.
Measured redshifts of emission and absorption lines.
| Line | zA | zC | zE |
|---|---|---|---|
| Lyα | 2.393 ± 0.006 | 2.391 ± 0.005 | – |
| Si IV+O IV | 2.380 ± 0.003 | 2.385 ± 0.004 | 2.37 ± 0.06 |
| C IV | 2.361 ± 0.003 | 2.368 ± 0.003 | 2.35 ± 0.04 |
| C III] | 2.364 ± 0.002 | 2.364 ± 0.002 | 2.369 ± 0.007 |
| C II | 2.383 ± 0.003 | 2.384 ± 0.006 | – |
| Mg II | 2.392 ± 0.004 | 2.395 ± 0.004 | 2.34 ± 0.04 |
| O I–1335 | 2.3843 ± 0.0005 | 2.3883 ± 0.0016 | |
| C II–1335 | 2.3843 ± 0.0005 | 2.3879 ± 0.005 | |
| Si II–1527 | 2.3841 ± 0.0005 | 2.3871 ± 0.0010 | |
| Fe II–1609 | 2.3851 ± 0.0010 | 2.3868 ± 0.0004 | |
| Al II–1671 | 2.3838 ± 0.0005 | 2.3866 ± 0.0005 | |
| Si II–1808 | 2.3835 ± 0.002 | 2.3849 ± 0.005 | |
| Fe II–2344 | 2.3848 ± 0.0004 | 2.3854 ± 0.0004 | |
| Fe II–2587 | 2.3830 ± 0.0005 | 2.3844 ± 0.0018 | |
| Fe II–2600 | 2.3834 ± 0.0009 | 2.3840 ± 0.0008 | |
Notes. Data are based on the extracted NOT spectra. The emission and absorption lines are shown above and below the line respectively. All uncertainties are statistical. Absolute and relative systematic uncertainties may exist at the level of ∼1 pixel, corresponding to 3 Å or a redshift uncertainty of 0.002 around C IV.
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