  We determine the fraction of F, G, and K dwarfs in the Solar Neighborhood
hosting hot jupiters as measured by the California Planet Survey from the Lick
and Keck planet searches. We find the rate to be 1.2\pm0.38%, which is
consistent with the rate reported by Mayor et al. (2011) from the HARPS and
CORALIE radial velocity surveys. These numbers are more than double the rate
reported by Howard et al. (2011) for Kepler stars and the rate of Gould et al.
(2006) from the OGLE-III transit search, however due to small number statistics
these differences are of only marginal statistical significance. We explore
some of the difficulties in estimating this rate from the existing radial
velocity data sets and comparing radial velocity rates to rates from other
techniques.
