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Table 2
Spectroscopic information of the four IFRS observed with FORS2.
| IFRS | z | Line | FWHM |
| ID | [km s-1] | ||
|
|
|||
| S212 | 2.76 ± 0.05 | C iv | 8700 ± 600 |
| 2.75 ± 0.02 | C iii] | 3300 ± 700 | |
| S265 | 1.85 ± 0.02 | C iv | 3900 ± 500 |
| 1.84 ± 0.02 | C iii] | 4200 ± 300 | |
| 1.84 ± 0.03 | Mg ii | 8400 ± 900 | |
| S713 | 2.13 ± 0.03 | C iv | 5400 ± 700 |
| 2.12 ± 0.03 | C iii] | 5900 ± 400 | |
| 2.13 ± 0.03 | Mg ii | 4600 ± 1000 | |
| S539 | – | – | – |
Notes. Listed are the IFRS ID, the spectrosopic redshift, and the emission line identified in the spectrum with the associated line width. We obtain the final redshift of each IFRS from the Mg ii emission line and from C iv where Mg ii was not available.
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