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We present radial velocity measurements of two stars observed as part of theLick Subgiants Planet Search and the Keck N2K survey. Variations in the radialvelocities of both stars reveal the presence of Jupiter-mass exoplanets inhighly eccentric orbits. HD 16175 is a G0 subgiant from the Lick SubgiantsPlanet Search, orbited by a planet having a minimum mass of 4.4 M_Jup, in aneccentric (e = 0.59), 2.71 yr orbit. HD 96167 is a G5 subgiant from the N2K("Next 2000") program at Keck Observatory, orbited by a planet having a minimummass of 0.68 M_Jup, in an eccentric (e = 0.71), 1.366 yr orbit. Both stars arerelatively massive (M_star = 1.3 M_sun) and are very metal rich ([Fe/H] >+0.3). We describe our methods for measuring the stars' radial velocityvariations and photometric stability.

Old, Rich, and Eccentric: Two Jovian Planets Orbiting Evolved Metal-Rich Stars