Table 3.
Properties of QSOs in our sample.
| QSO | z | log(MBH/M⊙) | log(Mdyn/M⊙) | SFR | GBH | GGAL | Angles | Class | Refs. |
|---|---|---|---|---|---|---|---|---|---|
| [M⊙ yr−1] | [10−8 yr−1] | [10−8 yr−1] | [deg] | ||||||
| J0100+2802 | 6.327 | 10.04 ± 0.27 | 10.51 ± 0.1 | 396 | 2.5 | 1.8 | 54 | BG (S) | [1], [2] |
| J036+03 | 6.540 | 9.49 ± 0.12 | 10.46 ± 0.1 | 466 | 1.1 | 1.8 | 31 | GG | [1], [2] |
| J0224−4711 | 6.522 | 9.36 ± 0.08 | 10.58 ± 0.3 | 2485 | 2.3 | 6.9 | 19 | GG | [1], [3] |
| J231−20 | 6.587 | 9.50 ± 0.09 | 10.15 ± 0.2 | 496 | 1.0 | 4.5 | 13 | GG | [1], [2] |
| J1342+0928 | 7.540 | 8.90 ± 0.14 | 10.56 ± 0.3 | 180 | 3.1 | 0.5 | 81 | BG | [1], [2] |
| J1148+5251 | 6.419 | 9.74 ± 0.03 | 10.18 ± 0.3 | 1570 | 1.1 | 16 | 4 | GG | [1], [4] |
| J2310+1855 | 6.003 | 9.67 |
10.72 ± 0.1 | 1855 | 1 | 4 | 15 | GG | [5], [6] |
| J2054−0005 | 6.390 | 9.17 ± 0.3 | > 10.46 | 730 | 1.1 | 2.7 | 23 | GG | [2] |
| J1319+0950 | 6.133 | 9.53 |
11.09 ± 0.1 | 1197 | 0.9 | 1.0 | 43 | S | [5], [2] |
| J183+05 | 6.439 | 9.41 |
> 11.11 | 894 | 1.0 | 0.7 | 54 | BG (S) | [5], [2] |
Notes. Columns: QSO name; redshift; BH mass; dynamical mass; SFR computed in Sect. 5.1; slope of the relation GBH − Ggal, exemplified by the slope of the arrows in Fig. 17; classification of the evolutionary state of each QSO; references for BH and dynamical masses. QSOs above the double black line belong to the HYPERION sample. SFRs are corrected by a factor of 50% to account for the possible contribution of the AGN to the dust heating (see Sect. 6.1.6). The dynamical mass for J0224−4711 was preliminarily estimated using the [CII] FWHM from an archival ALMA observations in band 6. This work is still in progress (Tripodi, in prep.). Classification: BG = BH growth regime, S = symbiotic growth regime, and GG = galaxy growth regime. J0100+2802 and J183+05 are classified twice; see text (Sect. 6.2).
References. [1] Zappacosta et al. (2023); [2] Neeleman et al. (2021); [3] Tripodi (in prep.); [4] Riechers et al. (2009); [5] Mazzucchelli et al. (2023); [6] Tripodi et al. (2022). For each line with multiple references, the first reference is for MBH and Lbol, which enters in ṀBH, and the second reference is for Mdyn.
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