Most recent update: June 26, 2013
The table below is available in ASCII format.
The original version of Table 3 in McConnell & Ma (2013) is also available in ASCII format.
| Galaxy | MBH (+,-) (Msun) |
σ (km/s) |
log(LV) | MV | log(L3.6) | M3.6 | Mbulge (Msun) |
Rinf (arcsec) | Reff V-band (arcsec) |
Reff i-band (arcsec) |
Reff 3.6um (arcsec) |
Distance (Mpc) | Morph | BH Mass Method |
BH Mass Reference |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Milky Way ^a | 4.1 (0.6,0.6) e6 | 103 ± 20 | — | — | — | — | — | 43.0 | — | — | — | 0.008 | S | stars | Ghez 2008, |
| A1836-BCG | 3.9 (0.4,0.6) e9 | 288 ± 14 | 11.26 ± 0.06 | -23.35 | — | — | — | 0.27 | — | 17.61 | — | 157.5 | E (C) | gas | Dalla Bonta 2009 |
| A3565-BCG ^b | 1.4 (0.3,0.2) e9 | 322 ± 16 | 11.24 ± 0.06 | -23.30 | — | — | — | 0.22 | — | — | — | 54.4 | E (C) | gas | Dalla Bonta 2009 |
| Circinus | 1.7 (0.4,0.3) e6 | 158 ± 18 | — | — | 10.31 ± 0.02 | -22.53 | — | 0.02 | — | — | 10.83 | 4.0 | S | masers | Greenhill 2003 |
| IC1459 ^b | 2.8 (1.1,1.2) e9 | 315 ± 16 | 10.96 ± 0.06 | -22.57 | 11.82 ± 0.12 | -26.30 | 3.07e11 | 0.81 | 29.8 | — | 61.1 | 30.9 | E (C) | stars | Cappellari 2002 |
| N221 (M32) | 2.6 (0.5,0.5) e6 | 75 ± 3 | 8.52 ± 0.02 | -16.47 | 8.95 ± 0.25 | -19.12 | 7.62e8 | 0.57 | 38.6 | — | 28.8 | 0.73 | E (I) | stars | Verolme 2002 |
| N224 (M31) | 1.4 (0.8,0.3) e8 | 160 ± 8 | — | — | — | — | 3.55e10 | 6.5 | — | — | — | 0.73 | S | stars | Bender 2005 |
| N524 | 8.6 (1.0,0.4) e8 | 235 ± 12 | 10.62 ± 0.04 | -21.74 | 11.26 ± 0.08 | -24.91 | — | 0.57 | — | — | 26.8 | 24.2 | S0 (C) | stars | Krajnovic 2009 |
| N821 | 1.7 (0.7,0.7) e8 | 209 ± 10 | 10.36 ± 0.05 | -21.10 | 11.28 ± 0.10 | -24.95 | 1.92e11 | 0.14 | 29.4 | 35.0 | 63.6 | 23.4 | E (I) | stars | Schulze 2011 |
| N1023 | 4.0 (0.4,0.4) e7 | 205 ± 10 | 10.06 ± 0.11 | -20.22 | 10.66 ± 0.07 | -23.41 | 6.49e10 | 0.08 | — | — | 24.0 | 10.5 | S0 (pl) | stars | Bower 2001 |
| N1194 | 6.8 (0.3,0.3) e7 | 148 ± (26,22) | — | — | — | — | — | 0.05 | — | — | — | 55.5 | S0 | masers | Kuo 2011 |
| N1277 | 1.7 (0.3,0.3) e10 | — | — | — | — | — | — | — | — | S0 | stars | van den Bosch 2012 | |||
| N1300 | 7.1 (3.4,1.8) e7 | 218 ± 10 | — | — | 10.55 ± 0.13 | -23.12 | — | 0.07 | — | — | 85.4 | 20.1 | S | gas | Atkinson 2005 |
| N1316 | 1.7 (0.3,0.3) e8 | 226 ± 11 | 11.18 ± 0.05 | -23.15 | 12.06 ± 0.32 | -26.91 | — | 0.14 | 65.8 | — | 93.0 | 21.0 | E (I) | stars | Nowak 2008 |
| N1332 | 1.5 (0.2,0.2) e9 | 328 ± 16 | 10.16 ± 0.05 | -20.60 | — | — | — | 0.54 | — | — | — | 22.7 | S0 (pl) | stars | Rusli 2011 |
| N1374 ^b | 5.9 (0.5,0.5) e8 | 174 ± 9 | 10.10 ± 0.05 | -20.43 | — | — | 5.54e10 | 0.89 | 25.4 | — | — | 19.6 | E (C) | stars | Rusli 2013 |
| N1399 ^b,c | 5.1 (0.6,0.7) e8 | 296 ± 15 | 10.78 ± 0.04 | -22.12 | — | — | 3.98e11 | 0.25 | 40.8 | — | — | 20.9 | E (C) | stars | Gebhardt 2007 |
| N1399 ^b,c | 1.3 (0.5,0.7) e9 | 296 ± 15 | 10.78 ± 0.04 | -22.12 | — | — | 3.98e11 | 0.25 | 40.8 | — | — | 20.9 | E (C) | stars | Houghton 2006 |
| N1407 ^b | 4.7 (0.9,0.5) e9 | 274 ± 14 | 11.05 ± 0.05 | -22.80 | — | — | 8.65e11 | 1.9 | 72.0 | — | — | 29.0 | E (C) | stars | Rusli 2013 |
| N1550 ^b | 3.8 (0.4,0.4) e9 | 289 ± 14 | 10.88 ± 0.05 | -22.36 | — | — | — | 0.76 | — | — | — | 53.0 | E (I) | stars | Rusli 2013 |
| N2273 | 7.8 (0.4,0.4) e6 | 144 ± (18,16) | — | — | — | — | — | 0.01 | — | — | — | 26.8 | S | masers | Kuo 2011 |
| N2549 | 1.4 (0.1,0.4) e7 | 145 ± 7 | 9.55 ± 0.04 | -19.04 | 10.18 ± 0.05 | -22.20 | 1.99e10 | 0.05 | 36.1 | — | 11.6 | 12.7 | S0 (pl) | stars | Krajnovic 2009 |
| N2787 | 4.1 (0.4,0.5) e7 | 189 ± 9 | — | — | 10.03 ± 0.23 | -21.82 | — | 0.14 | — | — | 15.7 | 7.5 | S0 (pl) | gas | Sarzi 2001 |
| N2960 | 1.21 (0.05,0.05) e7 | 166 ± (16,15) | — | — | — | — | — | 0.01 | — | — | — | 75.3 | S | masers | Kuo 2011 |
| N3031 (M81) | 8.0 (2.0,1.1) e7 | 143 ± 7 | — | — | 10.93 ± 0.12 | -24.06 | — | 0.85 | — | 94.6 | 127.3 | 4.1 | S | gas | Devereux 2003 |
| N3091 | 3.7 (0.1,0.2) e9 | 307 ± 15 | 11.02 ± 0.05 | -22.72 | — | — | — | 0.66 | 30.7 | — | — | 52.7 | E (C) | stars | Rusli 2013 |
| N3115 | 8.9 (5.1,2.7) e8 | 230 ± 11 | 10.34 ± 0.02 | -21.05 | 10.86 ± 0.04 | -23.90 | 1.57e11 | 1.58 | 47.4 | — | 27.3 | 9.5 | S0 (pl) | stars | Emsellem 1999 |
| N3227 | 1.5 (0.5,0.8) e7 | 133 ± 12 | — | — | 10.85 ± 0.20 | -23.88 | — | 0.04 | — | 59.1 | 82.9 | 17.0 | S | stars | Davies 2006 |
| N3245 | 2.1 (0.5,0.6) e8 | 205 ± 10 | — | — | 10.47 ± 0.08 | -22.93 | 7.00e10 | 0.21 | — | 26.7 | 4.6 | 21.5 | S0 (pl) | gas | Barth 2001 |
| N3368 | 7.6 (1.6,1.5) e6 | 122 ± (28,24) | — | — | 10.72 ± 0.04 | -23.56 | — | 0.04 | — | — | 45.6 | 10.6 | S | stars | Nowak 2010 |
| N3377 | 1.9 (1.0,1.0) e8 | 145 ± 7 | 9.93 ± 0.04 | -20.03 | 10.61 ± 0.07 | -23.28 | 2.35e10 | 0.69 | 35.2 | 59.5 | 55.2 | 11.0 | E (pl) | stars | Schulze 2011 |
| N3379 (M105) | 4.2 (1.0,1.1) e8 | 206 ± 10 | 10.29 ± 0.01 | -20.92 | 11.02 ± 0.07 | -24.30 | 6.86e10 | 0.83 | 43.3 | 57.0 | 46.0 | 10.7 | E (C) | stars | van den Bosch 2010 |
| N3384 | 1.1 (0.5,0.5) e7 | 143 ± 7 | 9.89 ± 0.09 | -19.92 | 10.18 ± 0.03 | -22.19 | 1.90e10 | 0.04 | 21.2 | 37.7 | 4.4 | 11.5 | E (pl) | stars | Schulze 2011 |
| N3393 | 3.3 (0.2,0.2) e7 | 148 ± 10 | — | — | — | — | — | 0.03 | — | — | — | 53.6 | S | masers | Kondratko 2008 |
| N3489 | 6.0 (0.8,0.9) e6 | 100 ± (15,11) | — | — | 10.14 ± 0.18 | -22.10 | — | 0.04 | — | — | 4.6 | 12.0 | S0 | stars | Nowak 2010 |
| N3585 | 3.3 (1.5,0.6) e8 | 213 ± 10 | 10.66 ± 0.08 | -21.82 | 11.04 ± 0.25 | -24.36 | 1.60e11 | 0.31 | 39.6 | — | 15.5 | 20.6 | S0 (I) | stars | Gultekin 2009 |
| N3607 | 1.4 (0.4,0.5) e8 | 229 ± 11 | — | — | 11.43 ± 0.06 | -25.34 | — | 0.10 | 36.1 | 36.4 | 44.6 | 22.6 | E (C) | stars | Gultekin 2009 |
| N3608 | 4.7 (1.0,1.0) e8 | 182 ± 9 | 10.34 ± 0.04 | -21.02 | 11.14 ± 0.09 | -24.60 | 7.66e10 | 0.55 | 29.7 | 28.4 | 56.4 | 22.8 | E (C) | stars | Schulze 2011 |
| N3842 ^b | 9.7 (3.0,2.5) e9 | 270 ± 14 | 11.20 ± 0.05 | -23.21 | — | — | 1.55e12 | 1.20 | 37.8 | — | — | 98.4 | E (C) | stars | McConnell 2011b |
| N3998 ^b | 8.5 (0.7,0.7) e8 | 272 ± 14 | 9.91 ± 0.04 | -19.97 | 10.35 ± 0.02 | -22.64 | — | 0.15 | — | 20.4 | 4.7 | 14.3 | S0 (pl) | stars | Walsh 2012 |
| N4026 | 1.8 (0.6,0.3) e8 | 180 ± 9 | 9.73 ± 0.08 | -19.52 | 10.32 ± 0.07 | -22.56 | 2.81e10 | 0.37 | 51.4 | 21.1 | 11.4 | 13.4 | S0 (pl) | stars | Gultekin 2009 |
| N4258 | 3.67 (0.01,0.01) e7 | 115 ± 10 | — | — | 10.88 ± 0.03 | -23.96 | — | 0.35 | — | 135.8 | 111.7 | 7.0 | S | masers | Herrnstein 2005 |
| N4261 | 5.3 (1.1,1.1) e8 | 315 ± 15 | 11.00 ± 0.02 | -22.67 | 11.43 ± 0.06 | -25.34 | 8.26e11 | 0.15 | 50.2 | 56.6 | 22.6 | 32.6 | E (C) | gas | Ferrarese 1996 |
| N4291 | 9.8 (3.1,3.1) e8 | 242 ± 12 | 10.25 ± 0.05 | -20.80 | — | — | 9.96e10 | 0.56 | 16.1 | — | — | 26.6 | E (C) | stars | Schulze 2011 |
| N4342 | 4.6 (2.6,1.5) e8 | 225 ± 11 | — | — | — | — | 1.80e10 | 0.35 | — | 7.6 | — | 23.0 | S0 (pl) | stars | Cretton 1999 |
| N4374 (M84) | 9.2 (1.0,0.8) e8 | 296 ± 14 | 10.98 ± 0.02 | -22.65 | 11.81 ± 0.02 | -26.28 | 3.62e11 | 0.51 | 64.8 | 53.8 | 105.9 | 18.5 | E (C) | gas | Walsh 2010 |
| N4388 | 8.8 (0.2,0.2) e6 | 107 ± (8,7) | — | — | — | — | — | 0.03 | — | — | — | 19.8 | S | masers | Kuo 2011 |
| N4459 | 7.0 (1.3,1.4) e7 | 167 ± 8 | 10.31 ± 0.02 | -20.98 | 10.63 ± 0.04 | -23.32 | — | 0.14 | — | 41.0 | 10.3 | 16.0 | E (pl) | gas | Sarzi 2001 |
| N4472 | 2.4 (0.3,0.1) e9 | 315 ± 16 | 11.04 ± 0.05 | -22.78 | — | — | 8.22e11 | 1.3 | 100.4 | — | — | 16.7 | E (C) | stars | Rusli 2013 |
| N4473 | 8.9 (4.5,4.4) e7 | 190 ± 9 | 10.29 ± 0.02 | -20.92 | 11.03 ± 0.02 | -24.32 | 1.61e11 | 0.15 | 30.3 | 34.8 | 49.3 | 15.2 | E (C) | stars | Schulze 2011 |
| N4486 (M87) ^b | 6.2 (0.3,0.4) e9 | 324 ± (28,16) | 11.08 ± 0.02 | -22.90 | 11.71 ± 0.02 | -26.01 | 1.31e12 | 3.14 | 100.4 | 68.4 | 99.5 | 16.7 | E (C) | stars | Gebhardt 2011 |
| N4486A | 1.4 (0.5,0.5) e7 | 111 ± 5 | 9.48 ± 0.02 | -18.90 | 10.21 ± 0.03 | -22.28 | — | 0.06 | — | 5.8 | 7.2 | 18.4 | E (pl) | stars | Nowak 2007 |
| N4526 | 4.73 (0.13,0.13) e8 | 222 ± 11 | — | — | — | — | — | 0.52 | — | 45.6 | — | 16.5 | S0 | gas | Davis 2013,Gould 2013 |
| N4564 | 8.8 (2.4,2.4) e7 | 162 ± 8 | — | — | 10.60 ± 0.05 | -23.25 | 4.66e10 | 0.19 | 31.7 | 22.4 | 25.0 | 15.9 | S0 (pl) | stars | Schulze 2011 |
| N4594 (M104) ^b | 6.7 (0.5,0.4) e8 | 230 ± 12 | 10.77 ± 0.06 | -22.10 | 11.10 ± 0.06 | -24.49 | 3.52e11 | 0.87 | — | — | 66.1 | 10.0 | S | stars | Jardel 2011 |
| N4596 | 8.4 (3.6,2.5) e7 | 136 ± 6 | — | — | 10.77 ± 0.02 | -23.68 | — | 0.22 | — | 56.2 | 28.0 | 18.0 | S0 (pl) | gas | Sarzi 2001 |
| N4649 (M60) ^b | 4.7 (1.1,1.0) e9 | 341 ± 17 | 10.99 ± 0.02 | -22.67 | 11.51 ± 0.04 | -25.54 | 7.72e11 | 2.18 | 76.1 | 67.5 | 47.1 | 16.5 | E (C) | stars | Shen 2010 |
| N4697 | 2.0 (0.2,0.2) e8 | 177 ± 8 | 10.46 ± 0.04 | -21.35 | 11.22 ± 0.04 | -24.79 | 1.29e11 | 0.46 | 79.5 | 59.7 | 100.5 | 12.5 | E (pl) | stars | Schulze 2011 |
| N4736 (M94) | 6.8 (1.6,1.6) e6 | 112 ± 6 | 9.76 ± 0.04 | -19.60 | — | — | — | 0.10 | — | — | — | 5.0 | S | stars | Kormendy 2011 |
| N4751 | 1.4 (0.1,0.1) e9 | 355 ± 18 | 10.26 ± 0.05 | -20.81 | — | — | — | 0.36 | — | — | — | 27.7 | E/S0 | stars | Rusli 2013 |
| N4826 (M64) | 1.6 (0.4,0.4) e6 | 96 ± 5 | 9.62 ± 0.04 | -19.25 | — | — | — | 0.02 | — | — | — | 7.3 | S | stars | Kormendy 2011 |
| N4889 ^b | 2.1 (1.6,1.55) e10 | 347 ± 17 | 11.48 ± 0.05 | -23.91 | — | — | 1.75e12 | 1.50 | 54.5 | — | — | 103.2 | E (C) | stars | McConnell 2011b |
| N5077 | 8.0 (5.0,3.3) e8 | 222 ± 11 | 10.75 ± 0.05 | -22.08 | 11.56 ± 0.10 | -25.65 | 3.66e11 | 0.32 | 25.0 | — | 29.2 | 44.9 | E (C) | gas | de Francesco 2008 |
| N5128 (Cen A)^d | 5.9 (1.1,1.0) e7 | 150 ± 7 | 10.60 ± 0.03 | -21.70 | 11.13 ± 0.11 | -24.57 | — | 0.60 | — | — | — | 4.1 | S0/E (C) | stars | Cappellari 2009 |
| N5328 | 4.8 (1.0,1.9) e9 | 333 ± 17 | 11.08 ± 0.05 | -22.86 | — | — | 1.18e12 | 0.58 | 21.7 | — | — | 65.9 | E | stars | Rusli 2013 |
| N5516 | 3.5 (0.2,0.4) e9 | 306 ± 26 | 11.10 ± 0.05 | -22.93 | — | — | — | 0.55 | — | — | — | 60.1 | E (C) | stars | Rusli 2013 |
| N5576 | 1.7 (0.3,0.4) e8 | 183 ± 9 | 10.39 ± 0.05 | -21.17 | 11.22 ± 0.06 | -24.79 | 9.58e10 | 0.18 | 28.9 | 49.4 | 34.3 | 25.7 | E (C) | stars | Gultekin 2009 |
| N5845 | 4.9 (1.5,1.6) e8 | 234 ± 11 | 9.75 ± 0.05 | -19.58 | 10.54 ± 0.01 | -23.11 | 3.36e10 | 0.31 | 3.3 | 4.3 | 3.7 | 25.9 | E (pl) | stars | Schulze 2011 |
| N6086 | 3.8 (1.7,1.2) e9 | 318 ± 16 | 11.23 ± 0.05 | -23.24 | — | — | 1.43e12 | 0.24 | 36.8 | — | — | 139.1 | E (C) | stars | McConnell 2011a |
| N6251 | 6.0 (2.0,2.0) e8 | 290 ± 14 | — | — | 12.07 ± 0.08 | -26.93 | 5.60e11 | 0.06 | — | — | 42.4 | 106.0 | E (pl) | gas | Ferrarese 1999 |
| N6264 | 3.03 (0.05,0.04) e7 | 158 ± (15,14) | — | — | — | — | — | 0.01 | — | — | — | 145.4 | S | masers | Kuo 2011 |
| N6323 | 9.8 (0.1,0.1) e6 | 158 ± (28,23) | — | — | — | — | — | 0.003 | — | — | — | 110.5 | S | masers | Kuo 2011 |
| N6861 | 2.1 (0.2,0.2) e9 | 389 ± 19 | 10.54 ± 0.05 | -21.51 | — | — | — | 0.43 | 22.8 | — | — | 28.9 | E/S0 | stars | Rusli 2013 |
| N7052 | 4.0 (2.8,1.6) e8 | 266 ± 13 | 10.92 ± 0.04 | -22.47 | 11.82 ± 0.06 | -26.29 | 3.50e11 | 0.07 | 40.5 | — | 39.3 | 70.9 | E (C) | gas | van der Marel |
| N7582 | 5.5 (1.6,1.1) e7 | 156 ± 19 | — | — | 11.06 ± 0.18 | -24.41 | — | 0.09 | — | — | 86.4 | 22.3 | S | gas | Wold 2006 |
| N7619 ^b | 2.6 (0.9,0.3) e9 | 313 ± 16 | 11.07 ± 0.05 | -22.85 | — | — | — | 0.44 | 34.3 | — | — | 53.9 | E (C) | stars | Rusli 2013 |
| N7768 ^b | 1.3 (0.5,0.4) e9 | 257 ± 13 | 11.09 ± 0.05 | -22.92 | — | — | 1.16e12 | 0.14 | — | — | — | 112.8 | E (C) | stars | McConnell 2012 |
| U3789 | 1.08 (0.06,0.05) e7 | 107 ± (13,12) | — | — | — | — | — | 0.02 | — | — | — | 48.4 | S | masers | Kuo 2011 |
| More Complicated Systems | MBH (+,-) (Msun) |
σ (km/s) |
log(LV) | MV | log(L3.6) | M3.6 | Mbulge (Msun) |
Rinf (arcsec) | Reff V-band (arcsec) |
Reff i-band (arcsec) |
Reff 3.6um (arcsec) |
Distance (Mpc) | Morph | BH Mass Method |
BH Mass Reference |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Cygnus A | 2.7 (0.7,0.8) e9 | 270 ± 14 | 10.43 ± 0.05 | -21.28 | — | — | — | 0.13 | — | — | — | 257.1 | E | gas | Tadhunter et al. 2003 |
| IC 2560 | 4.4 (4.4,2.2) e6 | 144 ± 7 | — | — | 10.88 ± 0.28 | -23.95 | — | 0.001 | — | — | 27.5 | 40.7 | S | masers | Ishihara 2001 |
| N1068 (M77) | 8.6 (0.3, 0.3) e6 | 151 ± 7 | — | — | 11.22 ± 0.02 | -24.79 | 2.36e10 | 0.02 | — | 44.5 | 9.8 | 15.4 | S | masers | Lodato 2003 |
| N1386 | 1.2 (1.1,0.6) e6 | 166 ± 8 | — | — | — | — | — | 0.002 | — | — | — | 16.1 | S0 | masers | Braatz 1997 |
| N2748 | 4.7 (2.0,1.9) e7 | 115 ± 5 | — | — | 10.24 ± 0.04 | -22.34 | — | 0.13 | — | — | 25.5 | 24.9 | S | gas | Atkinson 2005 |
| N3079 | 2.4 (2.4,1.2) e6 | 146 ± 7 | — | — | 11.18 ± 0.03 | -24.71 | — | 0.005 | — | — | — | 20.7 | S | masers | Trotter 1998,Yamauchi 2004,Kondratko 2005 |
| N4151 | 4.5 (0.5,0.5) e7 | 93 ± 5 | — | — | 10.33 ± 0.16 | -22.59 | — | 0.33 | — | — | 5.4 | 13.9 | S | stars | Onken 2007 |
| N4303 (M61) | 9.2 (8.6,8.6) e6 | 84 ± 4 | — | — | — | — | — | 0.06 | — | — | — | 17.9 | S | gas | Pastorini 2007 |
| N4350 | 5.6 (4.1,4.1) e8 | 181 ± 9 | — | — | — | — | — | 0.90 | — | — | — | 17.0 | S0 | gas,stars | Pignatelli 2001 |
| N4486B | 5.8 (2.9,2.0) e8 | 169 ± 8 | 9.07 ± 0.05 | -17.88 | — | — | — | 1.10 | — | — | — | 16.3 | E | stars | Kormendy 1997 |
| N4742 | 1.4 (0.4,0.5) e7 | 90 ± 5 | 9.84 ± 0.05 | -19.80 | — | — | — | 0.10 | 7.9 | — | — | 15.7 | E | stars | Tremaine 2002 |
| N4945 | 1.4 (0.7,0.5) e6 | 134 ± 7 | — | — | — | — | — | 0.02 | — | — | — | 3.7 | S | masers | Greenhill 1997 |
| N5055 | 8.5 (1.9,1.9) e8 | 101 ± 5 | — | — | — | — | — | 8.53 | — | — | — | 8.7 | S | gas | Blais-Ouellette 2004 |
| N5252 | 1.0 (1.6,0.46) e9 | 190 ± 10 | — | — | — | — | — | 0.24 | — | — | — | 103.7 | S0 | gas | Capetti 2005 |
| N5495 | 1.2 (1.2,0.6) e7 | — | — | — | — | — | — | — | — | — | — | 103 | Sb | masers | Kondratko 2006 |
| N5793 | 1.0 (1.0,1.0) e7 | — | — | — | — | — | — | — | — | — | — | 53.3 | Sb | masers | Hagiwara 2001 |
| N6240(S) | 1.6 (0.8,0.7) e9 | 282 ± (40,46) | — | — | — | — | — | 0.17 | — | — | — | 105.0 | Irr | stars | Medling 2011 |
| N7332 | 1.2 (0.6,0.4) e7 | 135 ± 7 | 9.72 ± 0.05 | -19.50 | — | — | — | 0.03 | 13.4 | — | — | 21.7 | S0 | stars | Haring & Rix 2004 |
| N7457 | 8.7 (5.2,5.2) e6 | 67 ± 3 | 9.30 ± 0.04 | -18.42 | 9.66 ± 0.36 | -20.89 | 6.19e9 | 0.14 | — | — | 13.85 | 12.2 | S0 (pl) | stars | Schulze 2011 |
Notes:
Last updated: June 26, 2013. Please cite McConnell & Ma (2013) if you use this website.
MBH (+,-) represents best-fit MBH and 1-σ errors.
3.6 micron magnitudes and luminosities are from Sani et al. (2011).
Distances use surface brightness fluctuations or assume H0 = 70 km/s/Mpc.
Morphologies are elliptical (E), lenticular (S0), spiral (S), and irregular (Irr). Inner photometric profiles are core (C), intermediate (I), and power-law (pl).
^a For the Milky Way’s bulge velocity dispersion, we adopt the value of Tremaine et al. (2002).
^b For several galaxies, we exclude kinematic data within rinf when computing σ. See Table 1 of McConnell & Ma (2013).
^c We include two black hole measurements for N1399, which appear individually reliable but are not mutually consistent.
^d The black hole mass in N5128 has been subject to numerous measurments, most of which are consistent. Here we use the latest stellar dynamical measurement.