Table 1.
Main properties of the six observed Type I QSOs in our sample.
| Target ID | RA | Dec | z | Lbol | Instr. | Seeing O III | Instr. | Seeing Lyα |
|---|---|---|---|---|---|---|---|---|
| (J2000) | (J2000) | [1047 erg s−1] | O III | [arcsec] | Lyα | [arcsec] | ||
| Q0050+0051 | 00:50:21.22 | +00:51:35.0 | 2.241 | 1.4 | ERIS | 0.54 | KCWI | 0.9 |
| Q0052+0140 | 00:52:33.67 | +01:40:40.8 | 2.297 | 2.9 | ERIS | 0.51 | KCWI | 0.8 |
| Q2121+0052 | 21:21:59.04 | +00:52:24.1 | 2.373 | 1.5 | ERIS | 0.60 | KCWI | 0.8 |
| Q2123-0050 | 21:23:29.46 | −00:50:52.9 | 2.282 | 7.5 | ERIS | 0.94 | KCWI | 1.0 |
| SDSSJ2319−1040 | 23:19:34.80 | −10:40:36.0 | 3.162 | 1.9 | ERIS | 0.95 | MUSE | 1.4 |
| SDSSJ1427−0029 | 14:27:55.85 | −00:29:51.1 | 3.359 | 3.2 | GNIRS | 0.8 | MUSE | 0.9 |
Notes. From left to right, the columns report the target’s name, right ascension and declination, spectroscopic redshift, bolometric luminosity, the instrument used to trace the [O III] λ5007 line, the seeing of such observations, the instrument used to trace the extended Lyα emission surrounding the quasars, and the seeing of such observations. The redshift z is estimated using the [O III] λ5007 line. The bolometric luminosity Lbol is computed using the monochromatic luminosity Lλ(1350 Å), and the bolometric correction factor given in Shen et al. (2011) and adapted from Richards et al. (2006): Lbol = 3.81 × λLλ(1350 Å). The obtained values can have up to 0.3 dex of intrinsic uncertainty.
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