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We present new bulge stellar velocity dispersion measurements for 10 activegalaxies with secure $M_{BH}$ determinations from reverberation-mapping. Thesenew velocity dispersion measurements are based on spatially resolved kinematicsfrom integral-field (IFU) spectroscopy. In all but one case, the field of viewof the IFU extends beyond the effective radius of the galaxy, and in the caseof Mrk 79 the field of view extends to almost one half the effective radius.This combination of spatial resolution and field of view allows for securedeterminations of stellar velocity dispersion within the effective radius forall 10 target galaxies. Spatially resolved maps of the first (V) and second($\sigma_{\star}$) moments of the line-of-sight velocity distribution (LOSVD)indicate the presence of kinematic substructure in most cases. In futureprojects we plan to explore methods of correcting for the effects of kinematicsubstructure in the derived bulge stellar velocity dispersion measurements.

The BRAVE Program - I: Improved Bulge Stellar Velocity Dispersion Estimates for a Sample of Active Galaxies