Table 2.
Fluxes and luminosities measured for the 5100 Å continuum, Hα and Hβ BLR lines, alongside the derived black hole masses and Eddington ratios using these properties.
| DELS J0411–0907 | VDES J0020–3653 | |
|---|---|---|
| F5100(10−18 erg s−1 cm−2 Å−1) | 1.40 ± 0.02 | 1.18 ± 0.01 |
| FHα(10−16 erg s−1 cm−2) |
 |
 |
| FHβ(10−16 erg s−1 cm−2) | 8.0 ± 0.3 |
 |
| λL5100(1046 erg s−1) | 3.2 ± 0.2 | 2.7 ± 0.2 |
| LHα(1044 erg s−1) |
 |
14.8 ± 0.1 |
| LHβ(1044 erg s−1) | 4.5 ± 0.2 | 4.7 ± 0.3 |
| MBH, Hβ, 5100(109 M⊙) (G) |
 |
 |
| MBH, Hβ, 5100(109 M⊙) (V) |
 |
 |
| MBH, Hβ(109 M⊙) (G) |
 |
 |
| MBH, Hβ(109 M⊙) (V) |
 |
 |
| MBH, Hα(109 M⊙) |
 |
 |
| LBol/LEdd, Hβ, 5100 (G) |
 |
 |
| LBol/LEdd, Hβ, 5100 (V) |
 |
0.4 ± 0.2 |
| LBol/LEdd, Hβ (G) |
 |
 |
| LBol/LEdd, Hβ (V) |
 |
0.2 ± 0.1 |
| LBol/LEdd, Hα |
 |
 |
Notes. The errors for the black hole masses and Eddington ratios include the fit uncertainties as well as the 0.43 dex uncertainty due to the intrinsic scatter in the scaling relations. We note that all flux uncertainties are measurement uncertainties and do not include any intrinsic uncertainty in the flux level from the data calibration. The two sets of MBH, Hβ, 5100 and MBH, Hβ and corresponding Eddington ratios refer to the calculations using Eqs. (3) and (4) for the Greene & Ho (2005) and Vestergaard & Peterson (2006) coefficients; these are marked with a ‘G’ and ‘V’ respectively.
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