Table 1.
Enlarged XQR-30 Sample: Redshift derived from the Mg II emission line modeling or, when available, from the [C II] emission line (see D’Odorico et al. 2023); C IV and Mg II full-width at half maximum; C IV blueshift (used in Eq. (4)); monochromatic luminosities at rest-frame 1350 Å and 3000 Å; bolometric luminosities; black hole masses and Eddington ratio values, derived from both the C IV and Mg II emission lines.
| Name | Redshift | FWHMCIV | FWHMMgII | C IV Blueshift | log λL1350 | log λL3000 | log Lbol | log MBH, CIV | log MBH, Mg II | λEdd,CIV | λEdd, Mg II |
|---|---|---|---|---|---|---|---|---|---|---|---|
| [km s−1] | [km s−1] | [km s−1] | [erg s−1] | [erg s−1] | [erg s−1] | [M⊙] | [M⊙] | ||||
| PSOJ007+04 (a) | 6.0015 ( † ) | 6169±1057 | 8176±473 | 2778±601 | 46.56 |
46.41 |
47.12 |
9.16 |
9.89 |
0.71±0.49 | 0.13±0.06 |
| PSOJ009–10 ( ‡ ,a) | 6.004 ( † ) | 8025±2963 | 7336±697 | 2956±456 | 46.42 |
46.63 |
47.34 |
9.28 |
9.9 |
0.88±0.73 | 0.21±0.06 |
| PSOJ023–02 ( ‡ ,a) | 5.90 | 4806±486 | 4065±201 | 832±112 | 46.39 |
46.62 |
47.33 |
9.37 |
9.39 |
0.7±0.26 | 0.68±0.12 |
| PSOJ025–11 (a) | 5.85 | 5283±1043 | 3976±196 | 1316±286 | 46.68 |
46.56 |
47.27 |
9.45 |
9.34 |
0.51±0.32 | 0.66±0.18 |
| PSOJ029–29 | 5.984 | 6886±1190 | 3501±292 | 2063±285 | 46.88 |
46.78 |
47.49 |
9.58 |
9.34 |
0.63±0.3 | 1.1±0.27 |
| ATLASJ029–36 | 6.02 | 5808±1517 | 3753±266 | 1924±377 | 46.73 |
46.38 |
47.1 |
9.39 |
9.2 |
0.4±0.26 | 0.6±0.1 |
| VDESJ0224–4711 | 6.526 | 5378±207 | 2863±206 | 1808±42 | 46.61 |
46.82 |
47.54 |
9.29 |
9.19 |
1.36±0.23 | 1.72±0.36 |
| PSOJ060+24 | 6.18 | 4522±625 | 3270±249 | 633±323 | 46.58 |
46.59 |
47.3 |
9.5 |
9.18 |
0.48±0.52 | 1.01±0.27 |
| J0408–5632 ( ‡ ) | 6.0345 | 6943±355 | 4057±323 | 2411±155 | 46.55 |
46.48 |
47.19 |
9.33 |
9.31 |
0.55±0.15 | 0.57±0.16 |
| PSOJ065–26 | 6.1871 ( † ) | 8866±2638 | 4878±836 | 3895±1503 | 46.83 |
46.64 |
47.35 |
9.41 |
9.56 |
0.67±0.66 | 0.48±0.17 |
| PSOJ065+01 ( ‡ ,a, b) | 5.79 | 2389±878 | 5569±849 | 2682±368 | 46.4 |
46.49 |
47.2 |
8.27 |
9.6 |
6.63±5.37 | 0.31±0.12 |
| PSOJ089–15 ( ‡ ) | 5.957 | 3345±707 | 4365±425 | 1385±164 | 46.6 |
46.86 |
47.57 |
8.99 |
9.57 |
2.94±1.48 | 0.77±0.18 |
| PSOJ108+08 | 5.9485 | 8164±628 | 4247±346 | 3109±281 | 46.84 |
46.75 |
47.46 |
9.48 |
9.49 |
0.74±0.26 | 0.72±0.24 |
| SDSSJ0842+1218 ( ‡ ) | 6.0754 ( † ) | 6041±270 | 3854±337 | 2078±37 | 46.58 |
46.54 |
47.25 |
9.3 |
9.3 |
0.68±0.11 | 0.68±0.15 |
| J0923+0402 ( ‡ ) | 6.633 ( † ) | 5940±327 | 3793±799 | 2682±135 | 46.5 |
46.79 |
47.51 |
9.11 |
9.42 |
1.92±0.45 | 0.95±0.44 |
| PSOJ158–14 | 6.0685 ( † ) | 6323±1538 | 3258±212 | 1767±1138 | 46.77 |
46.85 |
47.56 |
9.52 |
9.31 |
0.85±1.19 | 1.37±0.42 |
| PSOJ183+05 | 6.4386 ( † ) | 7075±2010 | 4476±1282 | 3035±348 | 46.69 |
46.49 |
47.2 |
9.29 |
9.41 |
0.62±0.47 | 0.48±0.36 |
| PSOJ183–12 ( ‡ ,a) | 5.86 | 6196±517 | 3203±517 | 3031±194 | 46.81 |
46.7 |
47.41 |
9.24 |
9.22 |
1.13±0.29 | 1.19±0.43 |
| PSOJ217–16 | 6.1498 ( † ) | 10292±909 | 2772±741 | 3243±1394 | 46.6 |
46.55 |
47.26 |
9.54 |
9.02 |
0.41±0.37 | 1.34±0.79 |
| PSOJ217–07 ( ‡ ) | 6.1663 | 9174±2402 | 2607±533 | 3260±2169 | 46.46 |
46.42 |
47.13 |
9.35 |
8.9 |
0.46±0.69 | 1.3±0.8 |
| PSOJ231–20 ( ‡ ) | 6.5869 ( † ) | 6470±241 | 4644±179 | 2528±116 | 46.74 |
46.65 |
47.36 |
9.34 |
9.52 |
0.79±0.12 | 0.53±0.07 |
| J1535+1943 | 6.370 ( † ) | 6268±654 | 5640±236 | 2353±271 | 46.51 |
46.88 |
47.6 |
9.23 |
9.8 |
1.78±0.77 | 0.48±0.15 |
| PSOJ239–07 ( ‡ ) | 6.1102 ( † ) | 4863±185 | 3947±79 | 537±63 | 46.72 |
46.74 |
47.46 |
9.68 |
9.42 |
0.46±0.17 | 0.83±0.24 |
| PSOJ242–12 (a) | 5.830 | 6791±1672 | 4892±495 | 1152±439 | 46.48 |
46.55 |
47.26 |
9.61 |
9.51 |
0.34±0.33 | 0.43±0.18 |
| PSOJ308–27 | 5.7985 | 5284±148 | 2852±131 | 535±115 | 46.7 |
46.64 |
47.35 |
9.74 |
9.09 |
0.32±0.14 | 1.4±0.26 |
| PSOJ323+12 | 6.5872 ( † ) | 2828±140 | 2450±284 | 326±27 | 46.65 |
46.56 |
47.27 |
9.26 |
8.92 |
0.78±0.19 | 1.73±0.5 |
| VIK J2211–3206 ( ‡ ) | 6.3394 ( † ) | 5114±224 | 3448±729 | 1811±97 | 46.66 |
46.73 |
47.44 |
9.27 |
9.3 |
1.15±0.2 | 1.06±0.47 |
| VDES J2250–5051 ( ‡ ) | 5.9767 | 16618±11883 | 5212±4022 | 3001±9685 | 46.58 |
46.73 |
47.44 |
9.99 |
9.66 |
0.22±1.45 | 0.46±0.72 |
| SDSSJ2310+18 ( ‡ ) | 6.0031 ( † ) | 8576±2362 | 5156±252 | 3224±1504 | 46.92 |
46.78 |
47.49 |
9.55 |
9.67 |
0.67±0.75 | 0.51±0.15 |
| PSOJ359–06 | 6.1722 ( † ) | 3257±142 | 2653±213 | 554±39 | 46.55 |
46.59 |
47.3 |
9.23 |
9.0 |
0.9±0.36 | 1.53±0.65 |
| SDSSJ0100+28 | 6.3268 ( † ) | 6647±1971 | 5742±1705 | 2496±316 | 47.58 |
47.44 |
48.15 |
9.82 |
10.1 |
2.94±1.48 | 0.77±0.52 |
| ATLASJ025–33 | 6.3373 ( † ) | 6408±962 | 3302±768 | 2461±251 | 47.03 |
46.95 |
47.66 |
9.51 |
9.37 |
0.88±0.73 | 0.21±0.7 |
| ULASJ0148+06 | 5.977 | 5811±368 | 4741±473 | 2906±129 | 46.85 |
46.74 |
47.46 |
9.23 |
9.58 |
0.7±0.26 | 0.68±0.13 |
| PSOJ036+03 | 6.5405 ( † ) | 10131±329 | 3872±367 | 3727±135 | 46.82 |
46.79 |
47.5 |
9.55 |
9.43 |
0.51±0.32 | 0.66±0.2 |
| QSOJ0439+1634 (c) | 6.5188 ( † ) | 5352±110 | 3329±295 | 1773±58 | 47.51 |
47.62 |
48.33 |
9.77 |
9.72 |
0.63±0.3 | 1.1±0.62 |
| SDSSJ0818+17 | 5.96 | 9869±805 | 5477±334 | 3727±329 | 46.86 |
46.85 |
47.56 |
9.55 |
9.76 |
0.4±0.26 | 0.6±0.13 |
| SDSSJ0836+00 | 5.773 | 6908±196 | 3793±691 | 573±77 | 47.06 |
47.14 |
47.85 |
10.15 |
9.59 |
1.36±0.23 | 1.72±0.51 |
| SDSSJ0927+20 | 5.7722 ( † ) | 5480±732 | 3405±243 | 1785±166 | 46.55 |
46.37 |
47.08 |
9.28 |
9.11 |
0.48±0.52 | 1.01±0.36 |
| SDSSJ1030+05 | 6.304 | 5002±391 | 3578±336 | 1092±92 | 46.64 |
46.61 |
47.32 |
9.45 |
9.27 |
0.55±0.15 | 0.57±0.31 |
| SDSSJ1306+03 | 6.033 ( † ) | 4567±688 | 3825±449 | 769±189 | 46.66 |
46.53 |
47.24 |
9.5 |
9.29 |
0.67±0.66 | 0.48±0.19 |
| ULASJ1319+09 | 6.1347 ( † ) | 6964±2636 | 4905±162 | 3150±2607 | 46.73 |
46.58 |
47.3 |
9.28 |
9.53 |
0.71±0.49 | 0.13±0.09 |
| CFHQSJ1509–1 | 6.1225 ( † ) | 5095±828 | 3586±707 | 1021±216 | 46.59 |
46.65 |
47.37 |
9.47 |
9.3 |
6.63±5.37 | 0.31±0.39 |
Notes. ( † ) Redshift from [C II] emission line (see D’Odorico et al. 2023). ( ‡ ) Classified as a BAL quasar (Bischetti et al. 2022). (a) Note: the Mg II emission line in this spectrum is very close to/within a strong telluric feature, therefore it needs to be taken with caution. (b) Note: the C IV emission line region in this spectrum has low S/N, therefore the derived black holes and Eddington ratios need to be taken with caution. (c) This quasar is gravitationally lensed (Fan et al. 2019): the values presented here are not corrected for magnification. This quasar was not included in the comparison with lower-z sources in the discussion session.
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