Monte Carlo sampling plot of the planet mass vs. the semimajor axis, with the ice line planet formation model (scenario A) in the left, the log-uniform distributed planet formation model (scenario B) in the right, α_t = 10⁻³ in the top and α_t = 10⁻⁴ in the bottom. The color corresponds to the stellar mass. Scenario A only produces close-in planets, while planets formed in scenario B have a wide range of orbital distances.