Table 1.
BH mass, half-light radius, I-band magnitudes, redshift, luminosity distance, and luminosity for the sources in the sample.
Name | log(MBH) | log(R1/2) | Icorr | z | DL | log(L3000) |
---|---|---|---|---|---|---|
(M⊙) | (cm) | (mag) | (Gpc) | (ergs s−1) | ||
QJ 0158 | 8.2 (a) | 15.14 ± 0.3 | 19.09 ± 0.12 | 1.290 | 9.3 | 45.32 ± 0.05 |
HE 0435 | 8.7 (a) | 15.94 ± 0.6 | 20.76 ± 0.25 | 1.689 | 13 | 44.94(45.10)±0.10 |
SBS 0909 | 8.5 (b) | 15.51 ± 0.30 (e) | − | 1.378 | – | – |
SDSS 0924 | 8.0 (a) | 15.24 ± 0.35 | 21.24 ± 0.25 | 1.523 | 11.4 | 44.64 ± 0.10 |
FBQ 0951 | 8.95 (a) | 16.34 ± 0.35 | 17.16 ± 0.11 | 1.246 | 8.9 | 46.00 ± 0.04 |
Q 0957 | 9.0 (b) | 16.42 ± 0.50 (e) | − | 1.416 | – | – |
SDSS 1004 | 8.6 (a) | 15.14 ± 0.3 | 20.97 ± 0.44 | 1.738 | 13.4 | 44.89(45.0)±0.18 |
HE 1104 | 9.4 (b) | 16.14 ± 0.25 | 18.17 ± 0.31 | 2.319 | 19.1 | 46.31 ± 0.12 |
PG 1115 | 9.1 (b) | 16.84 ± 0.35 | 19.52 ± 0.27 | 1.733 | 13.4 | 45.47 ± 0.11 |
RXJ 1131 | 7.8 (a) | 15.54 ± 0.2 | 20.73 ± 0.11 | 0.654 | 4.0 | 43.94 ± 0.04 |
SDSS 1138 | 7.7 (b) | 15.14 ± 0.6 | 21.97 ± 0.19 | 2.445 | 20.4 | 44.85 ± 0.08 |
SBS 1520 | 8.95 (a) | 15.94 ± 0.2 | 18.92 ± 0.13 | 1.855 | 14.5 | 45.78 ± 0.05 |
WFI 2033 | 8.6 (c) | 16.26 ± 0.30 (e) | − | 1.661 | – | – |
WFI 2026 | 9.4 (d) | 15.98 ± 0.31 (e) | − | 2.223 | – | – |
Q 2237 | 8.7. (b) | 15.84 ± 0.3 | 17.90 ± 0.44 | 1.695 | 13 | 46.09(46.3)±0.18 |
Notes.
BH mass measurements are taken from Morgan et al. (2010), and
When not available, we use the measurements of Sluse et al. (2012), and
The logarithm of R1/2 (third column) are taken from Morgan et al. (2010, except from (e) which are taken from Cornachione & Morgan 2020). Fourth column lists the (unmagnified) I-band magnitudes taken from Morgan et al. (2010). Redshift and luminosity distances (fifth and sixth column, respectively) are taken from NED, assuming H0 = 67.8 km s−1 Mpc−1, Ωmatter = 0.308, Ωvacuum = 0.692.
The NASA/IPAC Extragalactic Database (NED) is funded by the National Aeronautics and Space Administration and operated by the California Institute of Technology.
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