  We present a set of 109 new, high-precision Keck/HIRES radial velocity (RV)
observations for the solar-type star HD 32963. Our dataset reveals a candidate
planetary signal with a period of 6.49 $\pm$ 0.07 years and a corresponding
minimum mass of 0.7 $\pm$ 0.03 Jupiter masses. Given Jupiter's crucial role in
shaping the evolution of the early Solar System, we emphasize the importance of
long-term radial velocity surveys. Finally, using our complete set of Keck
radial velocities and correcting for the relative detectability of synthetic
planetary candidates orbiting each of the 1,122 stars in our sample, we
estimate the frequency of Jupiter analogs across our survey at approximately
3%.
