  We present Chandra observations of 12 galaxies that contain supermassive
black holes with dynamical mass measurements. Each galaxy was observed for 30
ksec and resulted in a total of 68 point source detections in the target
galaxies including supermassive black hole sources, ultraluminous X-ray
sources, and extragalactic X-ray binaries. Based on our fits of the X-ray
spectra, we report fluxes, luminosities, Eddington ratios, and slope of the
power-law spectrum. Normalized to the Eddington luminosity, the 2--10 keV band
X-ray luminosities of the SMBH sources range from $10^{-8}$ to $10^{-6}$, and
the power-law slopes are centered at $\sim2$ with a slight trend towards
steeper (softer) slopes at smaller Eddington fractions, implying a change in
the physical processes responsible for their emission at low accretion rates.
We find 20 ULX candidates, of which six are likely ($>90%$ chance) to be true
ULXs. The most promising ULX candidate has an isotropic luminosity in the
0.3--10 keV band of $1.0_{-0.3}^{+0.6} \times 10^{40}$ erg/s.
