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Table 1.

Sources analyzed in this paper.

Source z Type MBH (M⊙) log Lbol/(erg s−1) log λEdd
1H 0419-577 0.104 Sy1 2.2 × 108 45.68 −0.84
4C 50.55 0.02 RLSy1 9.3 × 107 44.91 −1.24
Ark 564 † 0.0243 NLSy1 3.2 × 106 45.00 0.39
ESO 103-G35 0.00914 Sy1 2.3 × 107 44.54 −1.01
ESO 362-G18 0.01244 Sy1.5 1.3 × 107 44.07 −1.22
ESO 383-G18 0.01241 Sy2 3.0 × 105 43.79 0.15
GRS 1734-292 0.021 Sy1 6.9 × 107 44.95 −1.07
HE 1143-1810 0.0329 Sy1 2.5 × 107 44.95 −0.62
IC4329A 0.01613 Sy1 4.5 × 107 45.06 −0.77
MCG-5-23-16 0.00823 Sy1 4.5 × 107 44.34 −1.49
MCG+8-11-11 0.02 Sy1 4.1 × 106 44.93 0.15
Mrk 6 0.01951 Sy1.5 1.3 × 108 44.52 −1.76
Mrk 110 0.03552 Sy1 1.9 × 107 45.06 −0.41
Mrk 509 0.01951 Sy1 1.1 × 108 45.27 −0.96
NGC 3281 0.01073 Sy2 1.7 × 108 44.06 −2.04
NGC 5506 0.00589 NLSy1 1.7 × 107 44.14 −1.24
NGC 5728 0.00947 Sy2 1.8 × 108 44.14 −2.28
NGC 6814 0.00523 Sy1 1.1 × 107 43.52 −1.7
SWIFT J2127.4+5654 0.0144 NLSy1 1.4 × 107 44.11 −1.22
UGC 6728 0.00652 Sy1 3.5 × 105 43.16 −0.57

Notes. The most common name, the redshift, the AGN type, the black hole mass (MBH), the bolometric luminosity (Lbol), and the Eddington ratio (λEdd) are listed in this table. All values of MBH, Lbol and λEdd are extracted from the BASS catalog published by Koss et al. (2022).

†The only exception is Ark 564, for which we retrieved a reverberation mapping mass estimate from Peterson et al. (2004), with Lbol estimated applying a bolometric correction to the X-ray luminosity.

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