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Table 1.

Key properties of the sample.

Source log(MBH) log(Lbol) νb Ref. νb RL RHβ Ref. RHβ
(M) (erg s−1) (10−6 Hz) (pc)
(1) (2) (3) (4) (5) (6) (7) (8)
1H0707-495( * ) 6.6 c 398 (1) l l l
2MASXJ23444 ( † ) 10.1 47.76 0.0225 (2) −3.99 l l
3C120( * ) 7.74 45.17 7.8 (2) −3.11 (1)
3C273 8.84 47.02 0.7 (2) −2.78 (2)
3C445 8.39 45.50 1.36 (2) −2.75 l l
4C+29.30 8.28 44.91 1.3 (2) −3.59 l l
4C+74.26 9.83 46.01 0.02 (2) −3.30 l l
Cen A 7.77 43.10 2.3 (2) −3.35 l l
Circinus Galaxy 6.23 43.55 107.15 (1) −4.50 l l
Cygnus A 9.43 45.56 0.05 (2) −0.73 l l
H1821+643 9.26 47.52 0.291 (2) −4.13 l l
IC 4329A( * ) 7.81 45.04 5.9 (2) −5.43 (1)
M 81 7.90 39.55 0.2 (2) −3.99 l l
MCG-6-30-15( * ) 6.14 43.86 38 (1) −6.59 l l
MR 2251-178 8.20 45.78 0.25 (1) −5.59 l l
MRK 1040 7.41 44.57 15.5 (2) −5.47 l l
MRK 1210 6.76 44.30 99.4 (2) −4.53 l l
MRK 273 8.78 44.13 0.2 (2) −3.70 l l
MRK 290 7.28 44.36 20.6 (2) −5.44 (3)
MRK 3 6.72 44.84 151.3 (2) −4.08 l l
MRK 509( * ) 8.05 45.26 0.08 (1) −5.50 (1)
MRK 766( * ) 6.962 43.91 290 (1) −4.52 l l
NGC 1068 6.93 43.94 48.1 (2) −3.07 l l
NGC 1275 7.55 45.14 13.8 (2) −2.36 l l
NGC 1365 7.84 43.44 2.2 (2) −3.99 l l
NGC 2992 8.33 43.13 0.4 (2) −3.85 l l
NGC 3393 7.52 43.80 7.2 (2) −5.06 l l
NGC 3516( * ) 7.39 43.85 6.6 (1) −5.36 (1)
NGC 3783( * ) 7.37 44.57 13 (1) −5.41 (1)
NGC 4051( * ) 6.13 42.42 510 (1) −4.40 (1)
NGC 4151( * ) 7.56 43.44 0.58 (1) −4.96 (1)
NGC 4388 6.94 44.22 54.4 (2) −5.23 l l
NGC 5548 7.72 44.34 1.3 (1) −5.23 (4)
NGC 6300 6.57 43.02 88 (3) l l l
NGC 7469 6.96 44.38 56.0 (2) −4.35 (1)
NGC 7582 7.74 44.66 5.9 (2) −4.63 l l
Pictor A 6.80 44.63 105.6 (2) −2.77 l l
PKS2153-69 7.23 44.23 22.6 (2) −1.49 l l

Notes. Col. (1): Object name. Sources denoted by ( * ) have potential relativistically broadened Kα components reported in the literature (e.g., Brenneman & Reynolds 2009; de La Calle Pérez et al. 2010; Zoghbi et al. 2010, 2012; Lohfink et al. 2013; Tzanavaris et al. 2019); additional care should be exercised when interpreting the fluxes as assessed from our simple continuum and narrow line model components for these sources (see Sect. 4.3 for details); Col. (2) Black hole mass obtained from Koss et al. (2017) and BASS DR2 (Koss et al. 2022); Col. (3) AGN bolometric luminosity obtained from Koss et al. (2017) and BASS DR2; Col. (4): Break frequency of the X-ray power spectrum; Col. (5): Reference for the νb, (1) refers to Summons (2007) and (2) refers to Eq. (6); Col. (6): Radio-loudness from Ricci et al. (2017a), defined as RL = log(F1.4 GHz/F14−150 keV); Col. (7): optical BLR radius (RHβ) calculated from Hβ reverberation lags; Col. (8): reference for RHβ, (1) refers to Bentz et al. (2009), (2) refers to Zhang et al. (2019), (3) refers to Du et al. (2016), and (4) refers to Lu et al. (2016). ( † ) 2MASXJ23444 refers to 2MASX J23444387-4243124.

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