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Table 6.
Broad emission lines properties derived from the fit of the NIR spectra shown in Fig. 3.
| Quasar Name | FWHM C IVcorr | FWHM Mg II | zC IV | C IVblueshift | C IV EW |
|---|---|---|---|---|---|
| km s−1 | km s−1 | km s−1 | Å | ||
| (1) | (2) | (3) | (4) | (5) | (6) |
| PSO J037−08 | 2900 ± 95 | 1925 ± 70 | 6.644 ± 0.002 | 3170 ± 40 | 11.5 ± 0.3 |
| PSO J041+06 | 1900 ± 20 | 5013 ± 5 | 6.084 ± 0.003 | 9730 ± 25 | 6.3 ± 0.1 |
| PSO J067−14 | 4570 ± 10 | 3555 ± 5 | 6.685 ± 0.001 | 1225 ± 3 | 30.45 ± 0.05 |
| PSO J162−01 | 4140 ± 10 | 3735 ± 5 | 6.588 ± 0.001 | 2673 ± 3 | 13.79 ± 0.02 |
| PSO J217+04 | 3134 ± 85 | 3546 ± 70 | 6.642 ± 0.002 | 2093 ± 32 | 5.3 ± 0.1 |
| PSO J289+50 | 3220 ± 35 | 2520 ± 26 | 6.786 ± 0.002 | 2655 ± 15 | 20.65 ± 0.14 |
| PSO J335−15 | 5648 ± 6 | 2617 ± 2 | 6.465 ± 0.001 | 1819 ± 4 | 18.61 ± 0.02 |
Notes. Col (1): Quasar name. Col (2–3): C IV and Mg II full width at half maximum. Col (4): C IV redshift estimate from the peak of the emission line. Col (5): C IV blueshift. Col (6): EW of the C IV BEL.
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