We present a spectroscopic survey of the newly discovered Canes Venatici dwarf galaxy using the Keck/DEIMOS spectrograph. Two stellar populations of distinct kinematics are found to be present in this galaxy: an extended, metal-poor component, of half-light radius 7.8+2.4 −2.1 arcmin, which has a velocity dispersion of 13.9+3.2 −2.5 km s −1, and a more concentrated (half-light radius 3.6+1.1 −0...
