Table 1
Adopted 2–10 keV Eddington ratio, black hole mass, distance, and references for the data.
Source | λ2−10keV | M | D | Refs. |
× 10-2 | 107M⊙ | (Mpc) | ||
|
||||
IC 4329a | 0.48 |
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68.4 | 1a, 2 |
NGC 4151 | 0.12 | 5.4 ± 1.8 | 19.0 | 3b, 4, 4 |
NGC 4258 | 0.00094 | 3.6 | 7.2 | 5c, 6, 7 |
NGC 5548 | 0.28 |
![]() |
72.7 | 8, 9 |
NGC 6814 | 0.15 |
![]() |
22.8 | 10d, 9, 11 |
NGC 6814∗ | 0.021 | 1.9 ± 0.4 | 22.8 | 10d,12,11 |
NGC 7213 | 0.014 |
![]() |
22.0 | 13, 14, 11 |
Cent. A | 0.012 | 5.5 ± 3.0 | 3.8 | 15, 16, 17 |
Circinus | 1.1–2.3 | 0.17 ± 0.03 | 4.2 | 18, 19, 11 |
NGC 1068 | 1.7 | 1.0 | 14.4 | 20, 21, 11 |
NGC 4945 | 1.8 | 0.14 | 3.6 | 22, 23, 24 |
Notes. The references are given in the order X-ray measurement, M, and (if available) distance. λ2−10keV given in the second column involves rescaling (based on the Swift/BAT data, see text) of the average intrinsic luminosity given in the reference by a factor of
Reference. (1) Brenneman et al. (2014); (2) Markowitz (2009); (3) Lubiński et al. (2010); (4) Hönig et al. (2014); (5) Reynolds et al. (2009); (6) Miyoshi et al. (1995); (7) Herrnstein et al. (1999); (8) Brenneman et al. (2012); (9) Pancoast et al. (2015); (10) Walton et al. (2013); (11) Tully (1988); (12) Bentz et al. (2009); (13) Lobban et al. (2010); (14) Schnorr-Müller et al. (2014); (15) Fukazawa et al. (2011); (16) Cappellari et al. (2009); (17) Harris et al. (2010); (18) Arévalo et al. (2014); (19) Greenhill et al. (2003); (20) Bauer et al. (2015); (21) Greenhill et al. (1996); (22) Puccetti et al. (2014); (23) Greenhill et al. (1997); (24) Tully et al. (2009).
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