Top: distributions of detected planets with radii between 0.5 and 2.5 R _⊕ and orbital periods between 0.5 and 10 days around M3–M5 dwarfs in our simulations. The results using the DC15 planet occurrence rates for early-M dwarfs are shown in blue, and the results using the HU19 enhanced planet occurrence rates for M3–M5 dwarfs are shown in orange. Bottom: cumulative distribution functions for the two distributions shown in the top panel.