Table 1.
Properties of the objects in our final sample.
| Object | z | log(LBol) | C IV Abs. Width |
|---|---|---|---|
| (erg s−1) | (km s−1) | ||
| J0542–2003 | 3.151* | 47.1 | 1700 |
| J0845+2127 | 2.576⋆ | 47.0 | 4100 |
| J0857+3149 | 2.901 | 46.7 | 9000 |
| J1021+3209 | 2.635* | 46.6 | 1100 |
| J1035+3253 | 2.694 | 46.1 | 10 600 |
| J1054+3158 | 2.676⋆ | 46.8 | 1300 |
| J1229+3316 | 3.032 | 47.0 | 1100 |
| J1426+3151 | 2.792⋆ | 46.5 | 6600 |
Notes. Redshifts marked with a * or ⋆ were incorrectly determined by the DESI pipeline due to misidentification of emission features. In these cases, the reported redshifts were either adopted from SDSS (Pâris et al. 2018, marked with a ⋆) or calculated independently by fitting the Si IV emission line (marked with a *).
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