Table 1.
Quasar properties.
| SDSS ID | z | DL | Scale | log L[OIII] | log Lbol | log L1.4 GHz | log MBH | log |
|---|---|---|---|---|---|---|---|---|
| SDSS | (Mpc) | (kpc/″) | (L⊙) | (erg s−1) | (W Hz−1) | (M⊙) | ||
| J023224.24–081140.2 | 0.1001 | 461 | 1.846 | 8.60 | 45.73 | 22.96 | 7.46 ± 0.33 | −0.33 ± 0.35 |
| J101043.36+061201.4 | 0.0977 | 449 | 1.807 | 8.68 | 45.81 | 24.37 | 8.36 ± 0.77 | −0.80 ± 0.78 |
| J110012.39+084616.3 | 0.1004 | 462 | 1.851 | 9.20 | 46.33 | 24.18 | 7.82 ± 0.44 | 0.04 ± 0.45 |
| J115245.66+101623.8 | 0.0699 | 315 | 1.335 | 8.72 | 45.85 | 22.67 | 7.91 ± 0.33 | −0.72 ± 0.35 |
| J135646.10+102609.0 | 0.1232 | 576 | 2.213 | 9.21 | 46.34 | 24.36 | 8.58 ± 0.34 | −1.03 ± 0.36 |
| J143029.88+133912.0 | 0.0851 | 388 | 1.597 | 9.08 | 46.21 | 23.67 | 8.19 ± 0.35 | −0.35 ± 0.37 |
| J150904.22+043441.8 | 0.1115 (*) | 517 | 2.028 | 8.56 | 45.69 | 23.81 | 8.27 ± 0.76 | −0.22 ± 0.77 |
Notes. The values of Lbol listed here were derived from the non-parametric measurements of the [OIII] luminosity from Reyes et al. (2008), using a bolometric correction factor of 3500 (Heckman et al. 2004). Rest-frame radio luminosities are calculated from integrated FIRST fluxes (Becker et al. 1995), assuming a spectral index α = −0.7. Black hole masses and Eddington ratios are from Kong & Ho (2018).
The redshift measured from the NIR spectrum of J1509 is z = 0.1118 (Ramos Almeida et al. 2019).
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