Planet formation grid at 0.25 AU. We show the final planet masses after 3 × 10⁶ years of evolution as a function of alpha viscosity and the time a planetary embryo is inserted in the disk. Left panel: power-law case with static irradiative heating. Right panel: standard model with a dust-sublimation front that causes a temperature cap. The contours in black show the final planet masses differing by orders of 0.5 dex.