As Fig. 3, but partitioned according to host star mass. In the biased synthetic population, the domination by low-mass planets on short to intermediate orbits is similar for all stellar masses, but giant planets occur only around stars with masses 0.5 M_⊙ and higher. In contrast, the subgiant and giant planets in the observed sample occur most frequently around less massive stars. GJ 3512b, the giant planet in the 0.1 M_⊙ panel, is particularly at odds with theoretical predictions. No simulated planets with M sin(i) > 10 M_⊙ occur in this stellar mass bin.