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Table A.1.

Properties of the AGNs used in this work.

Source z L14 − 195 keV λ L λ ( 5100 Å ) $ \lambda L_{\lambda}(\mathrm{5100\,\AA}) $ λLλ(12 μm) log Lbol, 14 − 195 keV log L bol , 5100 Å $ \log L_{\mathrm{bol, 5100\,\AA}} $ log Lbol, 12 μm log Lbol log MBH log λEdd
(erg s−1) (erg s−1) (erg s−1) (erg s−1) (erg s−1) (erg s−1) (erg s−1) (M⊙)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
3C 120 0.033 44.4 44.0 44.2 45.3 44.9 44.9 45.3 7.5 −0.29
3C 273 0.158 ... 45.9 45.7 ... 46.6 46.5 46.6 8.5 0.03
Akn 120 0.033 44.3 43.9 44.2 45.2 44.8 44.9 45.2 8.4 −1.40
ESO 323-G77 0.015 43.2 43.1 43.7 44.0 44.1 44.3 44.0 7.1 −1.20
GQ Com 0.165 44.9 44.6 ... 45.9 45.5 ... 45.9 8.3 −0.54
H0507+164 0.018 43.8 42.6 ... 44.7 43.6 ... 44.7 7.0 −0.41
HE 1029-1401 0.086 44.8 44.6 ... 45.8 45.5 ... 45.8 8.7 −1.08
IC 4329A 0.016 44.3 43.5 44.2 45.1 44.4 44.9 45.1 8.2 −1.13
IRAS 03450+0055 0.032 ... 43.9 ... ... 44.8 ... 44.8 7.8 −1.07
IRAS 09149-6206 0.057 44.4 45.0 45.0 45.3 45.8 45.7 45.3 8.1 −0.83
IRAS 13349+2438 0.108 ... 45.0 45.6 ... 45.8 46.3 45.8 7.8 −0.12
MCG+08-11-011 0.021 44.1 43.3 ... 45.0 44.3 ... 45.0 7.7 −0.82
MCG-6-30-15 0.008 43.0 41.6 43.1 43.7 42.7 43.7 43.7 6.6 −1.04
Mrk 110 0.035 44.2 43.7 ... 45.1 44.6 ... 45.1 7.1 −0.10
Mrk 1239 0.020 ... 44.5 44.1 ... 45.4 44.8 45.4 6.4 0.85
Mrk 231 0.042 ... 45.0 45.2 ... 45.8 45.9 45.8 7.9 −0.16
Mrk 335 0.026 43.5 43.8 ... 44.3 44.7 ... 44.3 6.9 −0.73
Mrk 509 0.034 44.5 44.2 44.3 45.4 45.1 45.0 45.4 8.2 −0.90
Mrk 590 0.026 43.5 43.5 43.6 44.2 44.4 44.3 44.2 7.6 −1.43
Mrk 6 0.019 43.7 43.6 ... 44.6 44.5 ... 44.6 8.0 −1.56
Mrk 744 0.009 42.5 41.8 ... 43.2 42.9 ... 43.2 7.4 −2.26
Mrk 79 0.022 43.7 43.7 ... 44.6 44.6 ... 44.6 7.8 −1.37
Mrk 817 0.031 43.8 43.7 ... 44.6 44.6 ... 44.6 8.1 −1.53
NGC 1365 0.005 42.7 41.9 42.8 43.4 43.0 43.4 43.4 6.3 −1.00
NGC 3227 0.004 42.6 42.2 42.2 43.3 43.2 42.8 43.3 7.1 −1.94
NGC 3516 0.009 43.3 42.8 ... 44.1 43.8 ... 44.1 7.8 −1.81
NGC 3783 0.010 43.6 43.0 43.6 44.4 44.0 44.2 44.4 7.6 −1.27
NGC 4051 0.002 41.7 41.9 42.2 42.3 43.0 42.7 42.3 5.7 −1.50
NGC 4151 0.003 43.1 42.1 42.9 43.9 43.2 43.5 43.9 7.7 −1.93
NGC 4593 0.008 43.2 42.6 43.0 43.9 43.6 43.6 43.9 7.3 −1.50
NGC 5548 0.017 43.8 43.3 43.3 44.6 44.3 44.0 44.6 8.2 −1.68
NGC 7469 0.016 43.6 43.5 43.9 44.5 44.4 44.5 44.5 7.6 −1.26
NGC 7603 0.029 44.0 44.4 ... 44.9 45.3 ... 44.9 8.4 −1.65
PDS 456 0.184 ... 46.3 45.9 ... 47.0 46.6 47.0 8.7 0.22
PG 0844+349 0.064 ... 44.2 44.0 ... 45.1 44.8 45.1 7.7 −0.69
PG 0953+414 0.234 ... 45.2 ... ... 46.0 ... 46.0 8.4 −0.55
PG 1613+658 0.121 44.7 44.8 ... 45.6 45.6 ... 45.6 8.8 −1.27
PGC 50427 0.024 43.4 43.1 ... 44.1 44.1 ... 44.1 7.3 −1.30
PGC 89171 0.027 43.5 43.9 ... 44.4 44.8 ... 44.4 7.6 −1.36
UGC 11763 0.063 ... 44.3 44.7 ... 45.2 45.4 45.2 7.3 −0.23
UGC 545 0.061 ... 44.5 45.0 ... 45.4 45.7 45.4 7.0 0.28
WPVS 48 0.037 ... 43.6 ... ... 44.5 ... 44.5 7.0 −0.57
Z 229-15 0.028 ... 42.9 ... ... 43.9 ... 43.9 6.9 −1.15

Notes. (1) Source name. (2) Redshift from NED. (3) X-ray 14−195 keV 70-month Swift-BAT survey catalogue (Baumgartner et al. 2013) (4) optical luminosity at 5100 Å λLλ(5100 Å) collected from the BASS catalogue (Koss et al. 2017). (5) 12 μm luminosity λLλ(12 μm) from Asmus et al. (2014). (6) Bolometric luminosity derived from L14 − 195 keV using Eq. A.1. (7) Bolometric luminosity derived from λ L λ ( 5100 Å ) $ \lambda L_{\lambda}({5100\,\AA}) $ using Eq. A.2. (8) Bolometric luminosity derived from λLλ(12 μm) using Eqs. A.3, A.4, and A.1. (9) The adopted bolometric luminosity in this work: Lbol, 14 − 195 keV is preferred; when it is unavailable, L bol , 5100 Å $ L_{\mathrm{bol, 5100\,\AA}} $ is adopted. (10) Black hole mass from GRAVITY Collaboration (2023). (11) Eddington ratio calculated from columns (9) and (10).

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