Table 3.
Bolometric and monochromatic luminosities of the HYPERION QSOs.
| Name | Lbol | λL2500 Å | λL3000 Å | λL4400 Å | λL5100 Å | E[B − V] | λEdd | λL1 keV |
|---|---|---|---|---|---|---|---|---|
| J1342+0928 | 47.05 ± 0.04 | 46.60 ± 0.02 | 46.46 ± 0.02 | 46.20 ± 0.05 | 46.14 ± 0.07 | 0.01 | 1.11 ± 0.38 | 44.93 ± 0.09 |
| J1007+2115 | 47.19 ± 0.07 | 46.75 ± 0.03 | 46.67 ± 0.02 | 46.50 ± 0.03 | 46.44 ± 0.04 | 0.03 | 0.81 ± 0.16 | 44.87 ± 0.18 |
| J1120+0641 | 47.22 ± 0.05 | 46.84 ± 0.05 | 46.76 ± 0.05 | 46.59 ± 0.01 | 46.49 ± 0.01 | 0.05 | 0.50 ± 0.28 | 45.19 ± 0.07 |
| J0038−1527 | 47.25 ± 0.06 | 46.87 ± 0.03 | 46.78 ± 0.03 | 46.53 ± 0.02 | 46.42 ± 0.03 | 0.03 | 1.00 ± 0.23 | 44.96 ± 0.16 |
| J0252−0503 | 47.00 ± 0.06 | 46.59 ± 0.04 | 46.48 ± 0.04 | 46.24 ± 0.04 | 46.15 ± 0.06 | 0.01 | 0.56 ± 0.08 | 44.95 ± 0.19 |
| J0020−3653 | 47.10 ± 0.06 | 46.69 ± 0.05 | 46.66 ± 0.04 | 46.46 ± 0.02 | 46.35 ± 0.03 | 0.02 | 0.58 ± 0.13 | 45.21 ± 0.09 |
| J0411−0907 | 47.17 ± 0.04 | 46.74 ± 0.02 | 46.66 ± 0.02 | 46.47 ± 0.02 | 46.43 ± 0.03 | 0.01 | 1.84 ± 0.24 | 44.82 ± 0.08 |
| J0244−5008 | 47.07 ± 0.04 | 46.58 ± 0.03 | 46.54 ± 0.02 | 46.41 ± 0.01 | 46.37 ± 0.02 | 0.01 | 0.77 ± 0.27 | 45.31 ± 0.05 |
| J231.6−20.8 | 47.13 ± 0.05 | 46.70 ± 0.04 | 46.59 ± 0.07 | 46.29 ± 0.06 | 46.21 ± 0.10 | 0.01 | 0.34 ± 0.15 | 44.73 ± 0.13 |
| J036.5+03.0 | 47.23 ± 0.04 | 46.79 ± 0.03 | 46.72 ± 0.03 | 46.50 ± 0.02 | 46.40 ± 0.03 | 0.0 | 0.44 ± 0.13 | 44.61 ± 0.14 |
| J0224−4711 | 47.47 ± 0.05 | 47.04 ± 0.02 | 47.04 ± 0.02 | 46.82 ± 0.01 | 46.75 ± 0.01 | 0.07 | 0.75 ± 0.19 | 45.35 ± 0.06 |
| J011+09 | 46.87 ± 0.04 | 46.39 ± 0.02 | 46.42 ± 0.02 | 46.06 ± 0.04 | 45.92 ± 0.05 | 0.01 | 0.42 ± 0.04 | 44.86 ± 0.11 |
| J1148+5251 | 47.48 ± 0.04 | 46.95 ± 0.02 | 46.91 ± 0.02 | 46.81 ± 0.01 | 46.76 ± 0.01 | 0.02 | 0.44 ± 0.05 | 45.30 ± 0.09 |
| J083.8+11.8 | 47.13 ± 0.04 | 46.71 ± 0.03 | 46.64 ± 0.03 | 46.48 ± 0.02 | 46.38 ± 0.03 | 0.01 | 0.51 ± 0.16 | 44.41 ± 0.07 |
| J0100+2802 | 47.99 ± 0.03 | 47.54 ± 0.03 | 47.57 ± 0.06 | 47.37 ± 0.01 | 47.32 ± 0.01 | 0.0 | 0.70 ± 0.11 | 45.79 ± 0.03 |
| J025−33 | 47.38 ± 0.04 | 46.93 ± 0.01 | 46.89 ± 0.01 | 46.69 ± 0.01 | 46.64 ± 0.01 | 0.01 | 0.52 ± 0.04 | 45.06 ± 0.14 |
| J0050+3445 | 47.24 ± 0.06 | 46.84 ± 0.02 | 46.78 ± 0.03 | 46.55 ± 0.01 | 46.51 ± 0.01 | 0.04 | 0.29 ± 0.06 | 44.76 ± 0.09 |
| J029−36 | 47.17 ± 0.06 | 46.66 ± 0.03 | 46.60 ± 0.02 | 46.48 ± 0.01 | 46.42 ± 0.01 | 0.02 | 0.17 ± 0.03 | 45.03 ± 0.09 |
Notes. Logarithm of bolometric and monochromatic luminosities of the HYPERION sample in units of [erg/s] derived from the lum-K13 best fit. Monochromatic luminosities are corrected for the E[B − V]. The Eddington ratios λEdd were computed assuming the MBH reported in Table 1. L1 keV was derived from the observed 0.3−7 keV fluxes by adopting the photon index Γ reported in Zappacosta et al. (2023) and Tortosa et al. (2024).
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