We report precise Doppler measurements of two stars , obtained at Lick Observatory as part of our search for planets orbiting intermediate–mass subgiants . Periodic variations in the radial velocities of both stars reveal the presence of substellar orbital companions . These two stars are notably massive with stellar masses of 1.80 M _ { \odot } and 1.64 M _ { \odot } , respectively , indicating that they are former A–type dwarfs that have evolved off of the main sequence and are now K–type subgiants . The planet orbiting \kappa CrB has a minimum mass M _ { P } \sin { i } = 1.8 M _ { Jup } , eccentricity e = 0.146 and a 1208 day period , corresponding to a semimajor axis a = 2.7 AU . The planet around HD 167042 has a minimum mass M _ { P } \sin { i } = 1.7 M _ { Jup } and a 412.6 day orbit , corresponding to a semimajor axis a = 1.3 AU . The eccentricity of HD 167042 b is consistent with circular ( e = 0.027 \pm 0.04 ) , adding to the rare class of known exoplanets in long–period , circular orbits similar to the Solar System gas giants . Like all of the planets previously discovered around evolved A stars , \kappa CrBb and HD 167042b orbit beyond 0.8 AU .