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Table 12.
Derived properties of the sample.
Object name | log(Lbol) | log(MBH) | L/LEdd |
---|---|---|---|
[erg s−1] | [M⊙] | ||
(1) | (2) | (3) | (4) |
Mrk 335 | 44.95 ± 0.03 | 7.78 ± 0.05 | 0.10 ± 0.01 |
Mrk 110 | 44.46 ± 0.03 | 7.48 ± 0.05 | 0.06 ± 0.01 |
Mrk 509 | 45.34 ± 0.03 | 8.21 ± 0.16 | 0.09 ± 0.03 |
Ark 564 | 44.25 ± 0.03 | 6.94 ± 0.06 | 0.14 ± 0.02 |
Mrk 478 | 45.32 ± 0.03 | 7.51 ± 0.04 | 0.43 ± 0.05 |
Ton 28 | 46.26 ± 0.03 | 8.26 ± 0.05 | 0.67 ± 0.10 |
I Zw 1 | 45.62 ± 0.03 | 7.45 ± 0.05 | 0.98 ± 0.12 |
LB 2522 | 46.03 ± 0.03 | 8.22 ± 0.06 | 0.43 ± 0.07 |
LEDA 51016 | 45.26 ± 0.03 | 7.75 ± 0.05 | 0.22 ± 0.02 |
PHL 1092 | 45.72 ± 0.03 | 7.71 ± 0.05 | 0.67 ± 0.12 |
Fairall 9 | 45.08 ± 0.03 | 8.14 ± 0.05 | 0.06 ± 0.01 |
Ark 120 | 45.40 ± 0.03 | 8.29 ± 0.04 | 0.09 ± 0.01 |
NGC 3783 | 44.52 ± 0.03 | 7.71 ± 0.05 | 0.04 ± 0.01 |
Notes. (1) Object’s common name. (2) Bolometric luminosity. (3) Mass of the SMBH at the center of the galaxy. (4) Eddington ratio associated with accretion onto the SMBH.
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