Table 5
EWs of detected absorption lines and 2σ upper limits on some undetected lines, the EW for the blended systems include the contributions from all lines.
| λ obs | λ rest | ID | z | E W rest | log N/cm-2 |
| [Å] | [Å] | [Å] | |||
|
|
|||||
| 4102.26 | 972.54 | Lyγ | 3.218 | 2.39 ± 0.10 | – |
| 4329.70 | 1025.72 | Lyβ | 3.221 | 2.92 ± 0.06 | – |
| 5131 | 1215.67 | Lyα | 3.221 | – | 20.00 ± 0.15 |
| (5254) | 1242.80 | N v | (3.221) | <0.09 | <13.66 |
| (5276) | 1250.58 | S ii | (3.221) | <0.08 | <14.71 |
| 5291.01 | 1253.81 | S ii | 3.220 | 0.05 ± 0.02 | 14.58 ± 0.25 |
| 5320.00 | 1259.52 | S ii | 3.221 | (1.32 ± 0.07) | – |
| 1260.42 | Si ii | 3.221 | blended | – | |
| 1260.53 | Fe ii | 3.221 | – | ||
| (5335) | 1264.74 | Si ii* | (3.221) | <0.10 | <12.76 |
| 5497.30 | 1302.17 | O i | 3.222 | 1.07 ± 0.05 | >15.15 |
| 5506.82 | 1304.37 | Si ii | 3.222 | 0.70 ± 0.21 | 15.87 ± 0.16 |
| (5559) | 1317.22 | Ni ii | (3.221) | <0.11 | <13.59 |
| 5634.24 | 1334.53 | C ii | 3.222 | 1.51 ± 0.10 | >15.55 |
| 5884.87 | 1393.76 | Si iv | 3.222 | 0.20 ± 0.08 | 13.50 ± 0.14 |
| 5923.05 | 1402.77 | Si iv | 3.222 | 0.12 ± 0.05 | 13.50 ± 0.14 |
| 6444.50 | 1526.71 | Si ii | 3.221 | 0.86 ± 0.04 | 15.87 ± 0.16 |
| 6539.58 | 1548.20 | C iv | 3.223 | 0.26 ± 0.08 | 14.10 ± 0.13 |
| 6546.39 | 1550.78 | C iv | 3.221 | 0.22 ± 0.09 | 14.10 ± 0.13 |
| 6790.24 | 1608.45 | Fe ii | 3.221 | 0.17 ± 0.03 | 14.28 ± 0.24 |
| 6800.38 | 1611.20 | Fe ii | 3.221 | <0.01 | – |
| 7052.62 | 1670.79 | Al ii | 3.221 | 1.02 ± 0.05 | 15.12 ± 0.18 |
| (7863) | 1862.79 | Al iii | (3.221) | <0.35 | <12.71 |
| (8552) | 2026.13 | Zn ii | (3.221) | <0.45 | <12.73 |
| (8679) | 2056.25 | Cr ii | (3.221) | <0.54 | <13.47 |
Notes. The column densities were derived from CoG fitted for S ii, Si ii, Fe ii, C iv, Si iv and Al ii. Si ii* denotes a fine-structure line. Upper and lower limits were determined by assuming the ions to lie on the linear part of the CoG. The Lyα column density is taken from Jakobsson et al. (2006b) and is based on the 600V grism.
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