Last updated: June 26, 2013. Please cite
McConnell & Ma (2013)
if you use this website.
(+,-) represents best-fit MBH
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
^a For the Milky Way's bulge velocity dispersion, we adopt the value of Tremaine et
^b For several galaxies, we exclude kinematic data within
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.