Table A.1.
Compilation of literature sources with O VI, N V, or N IV] emission lines.
| ID | z | O VI | N V | N IV] | Ref | |
|---|---|---|---|---|---|---|
| GS+14 | 5.55 | ✓ | ✓p | ✓ | This work | |
| AGN | Q0353-383 | 1.96 | ✓ | ✓ | ✓ | Baldwin et al. (2003) |
| DLS1053-0528 | 4.02 | × | ✓ | Glikman et al. (2007) | ||
| NDWFS1433 | 3.88 | ✓ | ✓ | Glikman et al. (2007) | ||
| UDS24561 | 3.21 | ✓ | × | × | Tang et al. (2021) | |
| 33 NL AGN | 2 − 3 | ✓ | ✓ | ✓ | Hainline et al. (2011) | |
| 12 Seyfert 2 | 0 − 4 | ✓60% | Dors et al. (2014) | |||
| 59 radio-galaxies | 0 − 4 | ✓25% | Dors et al. (2014) | |||
| 10 QSO2 | 0 − 4 | ✓70% | Dors et al. (2014) | |||
| S82-20 | 3.08 | ✓ | ✓ | Lin et al. (2022) | ||
| J1254+0241 | 1.8 | ✓ | ✓ | Dhanda et al. (2007) | ||
| J1546-5253 | 2.0 | ✓ | ✓ | Dhanda et al. (2007) | ||
| J1553+0056 | 2.63 | ✓p | × | Appenzeller et al. (2005) | ||
| 16 QSO | 2.4 − 3.8 | ✓26% | ✓ | Dietrich & Wilhelm-Erkens (2000) | ||
| 11 QSO | 3.9 − 5.0 | ✓73% | ✓ | ✓73% | Dietrich et al. (2003) | |
| PSO J006+39 | 6.61 | ✓ | × | Koptelova et al. (2019) | ||
| J1512+119 | 2.11 | ✓ | × | × | Borguet et al. (2012) | |
| J000239+255034 | 5.80 | ✓ | Fan et al. (2006) | |||
| 124 QSO stack | 5.6 − 6.7 | ✓ | Bañados et al. (2016) | |||
| 13 AGN stack | 2 − 3.8 | ✓ | ✓ | Le Fèvre et al. (2019) | ||
| galaxy | Lynx Arc | 3.36 | × | × | ✓ | Fosbury et al. (2003) |
| 31 stack EW[C II] > 20 | 2 − 3.8 | ✓ | ✓ | Le Fèvre et al. (2019) | ||
| 120 stack 10 < EW[C II] < 20 | 2 − 3.8 | ✓ | ✓ | Le Fèvre et al. (2019) | ||
| J141445+544631 | 5.42 | × | × | ✓ | McGreer et al. (2018) | |
| J160810+352809 | 0.03 | ✓p | Jaskot et al. (2017) | |||
| Ion3 | 4.0 | × | ✓p | × | Vanzella et al. (2018) | |
| 17 low mass galaxies stack | 1.4 − 2.9 | ✓ | ✓6% | Stark et al. (2014) | ||
| L* lensed galaxy | 3.5 | ✓ | ✓ | Patrício et al. (2016) | ||
| J0121+0025 | 3.24 | ✓p | ✓p | × | Marques-Chaves et al. (2021) | |
Notes. Each row refers to a single source, a collection of sources, or a stacked spectrum. In the first case, the ID columns refer to the source name, in the second case, to the number and type of the sources in the collection, and in the third case, to the number of sources included in the stack. O VI, N V, and N IV] report the detection (✓) or the nondetection (×) of the respective emission line. No symbol indicates that the line falls out of the spectral range. In case of a collection of sources, the percentage refers to the fraction of sources with a detection in the reported emission lines. Finally, p indicates that the line exhibits a P Cygni profile.
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