Phased Doppler velocities for HD 13445 (K1 V). The solid line is a Keplerian orbital fit with a period of 15.764 days, a semiamplitude of 379 m s⁻¹, and an eccentricity of 0.046, yielding a minimum (﹩M\mathrm{sin}\,i﹩) of 4.04 ﹩M_{\mathrm{J}\,}﹩ for the companion. The rms of the Keplerian fit is 3.7 m s⁻¹. A linear trend of −108.1 m s⁻¹ yr⁻¹ has been removed from these velocities. These results are consistent with Queloz et al. (2000), with the possible exception of the linear trend.