Table 3
Black hole masses as measured and as estimated from the fundamental plane of black holes.
| Source | MBH | MBH,Merloni | MBH,Koerding | MBH,Gültekin | MBH,Bonchi | MBH,Nisbet | Ledd |
| [M⊙] | [M⊙] | [M⊙] | [M⊙] | [M⊙] | [M⊙] | 1046 [erg s-1] | |
|
|
|||||||
| 0208-512 | 8.8 | 5.7 ± 0.9 | 6.7 ± 1.0 | 7.4 ± 0.4 | 8.8 ± 1.3 | 4.06 ± 0.04 | 9.1 |
| 0244-470 | 5.1 ± 2.6 | 6.2 ± 2.7 | 7.2 ± 1.2 | 8 ± 4 | 3.08 ± 0.24 | ||
| 0402-362 | 5.2 ± 2.7 | 6.3 ± 2.7 | 7.3 ± 1.3 | 8 ± 4 | 2.9 ± 0.4 | ||
| 0426-380 | 8.6 | 6.0 ± 1.3 | 7.0 ± 1.5 | 7.6 ± 0.6 | 9.1 ± 1.9 | 4.49 ± 0.04 | 5.2 |
| 0447-439 | 8.8 | 2.5 ± 2.0 | 3.4 ± 1.5 | 6.2 ± 1.0 | 4.3 ± 2.5 | 0.3 ± 0.5 | 7.8 |
| 0506-612 | 5.7 ± 1.5 | 6.7 ± 1.6 | 7.4 ± 0.7 | 8.8 ± 2.1 | 4.14 ± 0.05 | ||
| 0521-365 | 3.6 ± 1.2 | 4.6 ± 1.1 | 6.6 ± 0.6 | 5.6 ± 1.6 | 1.67 ± 0.17 | ||
| 0537-441 | 9.3 | 6.4 ± 1.1 | 7.4 ± 1.4 | 7.7 ± 0.5 | 9.8 ± 1.7 | 5.05 ± 0.04 | 26.0 |
| 0637-752 | 5.7 ± 1.5 | 6.7 ± 1.6 | 7.5 ± 0.7 | 9.2 ± 2.1 | 4.409 ± 0.027 | ||
| 1057-797 | 8.8 | 5.8 ± 2.5 | 6.8 ± 2.8 | 7.5 ± 1.1 | 9 ± 4 | 4.27 ± 0.04 | 7.8 |
| 1424-418 | 6.0 ± 1.1 | 7.1 ± 1.2 | 7.6 ± 0.5 | 9.0 ± 1.5 | 3.98 ± 0.06 | ||
| 1440-389 | 1.9 ± 2.0 | 2.8 ± 1.4 | 5.9 ± 1.1 | 3.7 ± 2.5 | −0.1 ± 0.5 | ||
| 1454-354 | 9.3 | 6.0 ± 1.8 | 7.0 ± 2.0 | 7.6 ± 0.8 | 9.2 ± 2.6 | 4.567 ± 0.009 | 26.0 |
| 1610-771 | 5.9 ± 2.6 | 6.9 ± 2.8 | 7.5 ± 1.1 | 9 ± 4 | 4.35 ± 0.08 | ||
| 1954-388 | 5.7 ± 2.5 | 6.7 ± 2.8 | 7.4 ± 1.1 | 9 ± 4 | 4.408 ± 0.017 | ||
| 2005-489 | 8.7 | 3.1 ± 2.7 | 4.0 ± 2.2 | 6.4 ± 1.3 | 5 ± 4 | 1.1 ± 0.5 | 6.5 |
| 2052-474 | 6.1 ± 2.6 | 7.1 ± 2.9 | 7.6 ± 1.1 | 9 ± 4 | 4.39 ± 0.06 | ||
| 2142-758 | 5.5 ± 2.6 | 6.5 ± 2.7 | 7.4 ± 1.2 | 9 ± 4 | 3.85 ± 0.13 | ||
| 2149-306 | 5.3 ± 1.6 | 6.3 ± 1.6 | 7.4 ± 0.8 | 8.9 ± 2.2 | 3.58 ± 0.13 | ||
Notes. All values are given as log 10(M). Columns: (1) IAU B1950 name; (2) MBH from Ghisellini et al. (2009); MBH estimated after (3) Merloni et al. (2003); (4) Körding et al. (2006); (5) Gültekin et al. (2009); (6) Bonchi et al. (2013); (7) Nisbet & Best (2016); and (8) Eddington luminosity for the measure black hole mass, assuming isotropic emission. The black hole mass estimates include the uncertainties from the parameters, not the uncertainties in luminosities, as these are much smaller.
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