  Compared to planets around Sun-like stars, relatively little is known about
the occurrence rate and orbital properties of planets around stars more massive
than 1.3 Msun. The apparent deficit of planets around massive stars is due to a
strong selection bias against early-type dwarfs in Doppler-based planet
searches. One method to circumvent the difficulties inherent to massive
main-sequence stars is to instead observe them after they have evolved onto the
subgiant branch. We show how the cooler atmospheres and slower rotation
velocities of subgiants make them ideal proxies for F- and A-type stars. We
present the early results from our planet search that reveal a paucity of
planets orbiting within 1 AU of stars more massive than 1.5 Msun, and evidence
of a rising trend in giant planet occurrence with stellar mass.
