On the newly discovered Canes Venatici II dSph galaxy

We report on the detection of variable stars in the Canes Venatici II (CVn II) dwarf spheroidal galaxy, a new satellite of the Milky Way recently discovered by the Sloan Digital Sky Survey. We also present a V, B - V color-magnitude diagram that reaches V similar to 25.5 mag, showing the galaxy's main-sequence turnoff at V similar to 24.5 mag and revealing several candidate blue straggler stars. Two RR Lyrae stars have been identified within the half-light radius of CVn II, a fundamental-mode variable (RRab) with period P(ab) = 0.743 days, and a first- overtone (RRc) RR Lyrae star with P(c) = 0.358 days. The rather long periods of these variables along with their P c position on the period-amplitude diagram support an Oosterhoff type II classification for CVn II. The average apparent magnitude of the RR Lyrae stars, < V > = 21.48 +/- 0.02 mag, is used to obtain a precision distance modulus of mag and a corresponding distance of 160(-5)(+4) kpc, for an adopted reddening E(B - V) = 0.015 mag.