Table 4
Luminosity at 5100 Å, bolometric luminosity, SMBH mass, and Eddington ratio of the five WISSH quasars.
| SDSS | λL5100 Å | LBol |
|
|
λ Edd |
| (1) | (2) | (3) | (4) | (5) | (6) |
|
|
|||||
| J0745+4734 | 1.8 | 10.0 | 15.7±2.1 | 8.7±0.5 | 0.5±0.1 |
| J0900+4215 | 1.7 | 8.3 | 2.1±0.3 | 6.6±0.4 | 3.1±0.5 |
| J1201+1206 | 1.2 | 5.9 | 6.5±0.6 | 6.2±0.2 | 0.7±0.1 |
| J1326-0005 | 1.0 | 5.6 | 2.1±0.3 | 0.11 ±0.02 | 2.1 |
| J1549+1245 | 1.3 | 6.5 | 12.6±2.2 | 1.9±0.5 | 0.4±0.1 |
Notes. Columns give the following information: (1) SDSS ID; (2) intrinsic luminosity at 5100 Å (in units of 1047 erg s-1); (3) bolometric luminosity (in units of 1047 erg s-1); (4) Hβ-based SMBH mass (in units of 109M⊙); (5) CIV-based SMBH mass (in units of 109M⊙) listed in Weedman et al. (2012); and (6) Eddington ratio, as derived from our Hβ-based SMBH mass estimates. The error associated with the includes both the statistical uncertainties affecting the λLλ(5100 Å) and FWHM
values and the systematic uncertainty in the virial relation itself (~0.3 dex; see Bongiorno et al. 2014, for a complete discussion).
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