Azimuthally averaged radial profiles in our nominal simulation with a Jupiter-mass planet. Top: vertically integrated surface density of gas and large dust. Bottom: midplane temperature (primary vertical axis) and aspect ratio (secondary vertical axis). We show the final state after the hydrostatic relaxation (dotted black curve), the hydrodynamic relaxation (solid blue curve), and the main stage with the embedded planet (solid red curve). The planet location is marked with the dashed vertical line.