Doppler velocities for HD 52265. The rms to the best‐fit Keplerian (solid line) is 2.2 m s﹩^{-1}﹩, slightly better than the measurement error of 3.5 m s﹩^{-1}﹩. The period is 118.96 days, and the semiamplitude is 45 m s﹩^{-1}﹩. Assuming the mass of HD 52265 is 1.13 M﹩_{\odot }﹩, the minimum (﹩M\mathrm{sin}\,i﹩) mass of the companion is 1.13 M﹩_{\mathrm{J}\,}﹩, and the semimajor axis is 0.49 AU.