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Table 2

Spectral parameters, masses, luminosity, and accretion rates of the sources in the selected sample.

Source Ref. Γ Ec log(Mbh∕M⊙) Ref. Lbol∕LEdd L2–10 keV F2–10 keV kTe τ Geom. Model
[keV] ergs s−1 erg cm−2 s −1 [keV]
NGC 5506 1 1.91 ± 0.03 8.0 ± 0.2 (A) 0.006 0.053 6.2 Slab COMPTT
Sphere COMPTT
MCG-05-23-16 2 1.85 ± 0.01 170 ± 5 7.7 ± 0.2 (B) 0.058 0.18 10.4 30 ± 2 1.2 ± 0.1 Slab COMPTT
25 ± 2 3.5 ± 0.02 Sphere COMPTT
SWIFT J2127.4 3–4 2.08 ± 0.01 7.2 ± 0.2 (J) 0.136 0.14 2.9 Slab COMPTT
Sphere COMPTT
IC4329A 5–6 1.73 ± 0.01 185 ± 15 8.08 ± 0.3 (N) 0.125 0.56 12.0 37 ± 7 1.3 ± 0.1 Slab COMPTT
33 ± 6 3.4 ± 0.5 Sphere COMPTT
3C390.3 7 1.70 ± 0.01 120 ± 20 8.4 ± 0.4 (H) 0.241 1.81 4.03 40 ± 20 Sphere COMPTT
3C382 8 1.68 ± 0.03 9.2 ± 0.5 (D) 0.072 2.34 2.9 330 ± 30 0.2 ± 0.02 Slab COMPTT
GRS 1734-292 9 1.65 ± 0.05 53 ± 10 8.5 ± 0.1 (L) 0.036 0.056 2.9 12 ± 1 2.9 ± 0.2 Slab COMPTT
6.3 ± 0.3 Sphere COMPTT
NGC 6814 10 1.71 ± 0.04 7.0 ± 0.1 (C) 0.003 0.021 0.2 2.5†± 0.5 Sphere NTHCOMP
MCG +8-11-11 10 1.77 ± 0.04 7.2 ± 0.2 (E) 0.754 0.51 5.6 1.9†± 0.4 Sphere NTHCOMP
Ark 564 11 2.27 ± 0.08 42 ± 3 6.8 ± 0.5 (H) 1.313 0.39 – 15 ± 2 2.7†± 0.2 Sphere NTHCOMP
PG 1247+267 12–13 2.35 ± 0.09 8.9 ± 0.2 (M) 0.024 0.79 0.05 1.4†± 0.3 Sphere NTHCOMP
Ark 120 14–15 1.87 ± 0.02 8.2 ± 0.1 (H) 0.085 0.92 2.3 – – – –
NGC 7213 16 1.84 ± 0.03 > 140 8.0 ± 0.2 (G) 0.001 0.012 1.3 0.2 ± 0.1 Sphere COMPPS
MCG 6-30-15 17–18 2.06 ± 0.01 > 110 6.4 ± 0.1 (E) 0.238 0.056 5.5 – – – –
NGC 2110 19 1.65 ± 0.03 > 210 8.3 ± 0.2 (K) 0.016 0.35 12.5 190 ± 130 0.2 ± 0.1 Slab COMPTT
Mrk 335 21–22 2.14 ± 0.03 > 174 7.2 ± 0.1 (H) 0.284 0.18 1.9 – – – –
Fairall 9 20 1.95 ± 0.02 > 242 8.1 ± 0.7 (H) 0.054 0.60 2.9 – – – –
Mrk 766 17–23–24 2.22 ± 0.03 > 441 6.3 ± 0.1 (I) 1.254 0.046 1.4 – – – –
PG 1211+143 26 2.51 ± 0.2 > 124 8.2 ± 0.2 (H) 0.047 0.35 1.0 – – – –

Notes. Accretion rates are computed using the Lx in the 2–10 keV energy band using the bolometric correction of Marconi et al. (2004). Luminosity is in units of 1044 ergs s−1. Flux is in units of 10−11 erg cm−2 s −1. The bottom part of the table is for objects with lower values of the high-energy cut-off. (†) Estimated parameter.

References. 1. Matt et al. (2015), 2. Baloković et al. (2015), 3. Marinucci et al. (2014a), 4. Malizia et al. (2008), 5. Bianchi et al. (2009b), 6. Brenneman et al. (2014), 7. Lohfink et al. (2015), 8. Ballantyne et al. (2014), 9. Tortosa et al. (2017), 10. Tortosa et al. (2018), 11. Kara et al. (2017), 12. Lanzuisi et al. (2016), 13. Trevese et al. (2014), 14. Matt et al. (2014), 15. Porquet et al. (2018), 16. Ursini et al. (2015), 17. Marinucci et al. (2014b), 18. Emmanoulopoulos et al. (2014), 19. Marinucci et al. (2015), 20. Lohfink et al. (2016), 21. Parker et al. (2014), 22. Bianchi et al. (2001), 23. Buisson et al. (2017), 24. Risaliti et al. (2011), 25. Zoghbi et al. (2015), 26. Lawson & Turner (1997). Mass References. A. Papadakis (2004), B. Onori et al. (2017), C. Pancoast et al. (2014, 2015), D. Winter et al. (2009), E.Bian & Zhao (2003), F. Zhang & Wang (2006), G. Woo & Urry (2002), H. Peterson et al. (2004), I. Bentz et al. (2010), J. Halpern (2006), K. Moran et al. (2007), L. Tortosa et al. (2017), M. Trevese et al. (2014), N de La Calle Pérez et al. (2010).

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