Table 2
Equivalent widths and outflow velocities for the four galaxies with highest S/N absorption lines.
| Source ID | EW | v out | ||||||
|
( km s-1) | |||||||
|
|
||||||||
| N v1238 | N v1242 | C ii1335 | Si iv1393 | Si iv1403 | C iv1548 | C iv1551 | ||
|
|
||||||||
| 30555 | – | – | 0.41 ± 0.13 | 1.84 ± 0.10 | 2.27± 0.19 | 2.39 ± 0.33 a | 2.39± 0.33a | 480 ± 102 |
| 34743 | 1.35 ± 0.18 | 0.82 ± 0.08 | 1.45 ± 0.07 | – | – | – | – | 651 ± 64 |
| 38729 | – | – | 2.12 ± 0.32 | 2.54 ± 0.33 | 2.50 ± 0.45 | 0.67 ± 0.28 | 0.23 ± 0.15 | 547 ± 81 |
| 95692 | 11.20 ± 0.30 a | 11.20 ± 0.30 a | 0.66 ± 0.10 | – | – | – | – | 1518 ± 146 |
Notes. Column 1 contains the source ID, and Cols. 2 to 8 list the measured EW for the lines seen in the spectra. In the last column the outflowing velocities measured using vpfit are given, for which the errors are calculated based on the analysis of 1000 mock spectra obtained from each galaxy spectrum.
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