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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 candidateplanetary signal with a period of 6.49 $\pm$ 0.07 years and a correspondingminimum mass of 0.7 $\pm$ 0.03 Jupiter masses. Given Jupiter's crucial role inshaping the evolution of the early Solar System, we emphasize the importance oflong-term radial velocity surveys. Finally, using our complete set of Keckradial velocities and correcting for the relative detectability of syntheticplanetary candidates orbiting each of the 1,122 stars in our sample, weestimate the frequency of Jupiter analogs across our survey at approximately3%.

The Lick-Carnegie Exoplanet Survey: HD32963 -- A New Jupiter Analog Orbiting a Sun-like Star