Heat maps of simulations with the Birnstiel et al. (2018) D-50 opacities with 50% porostiy. From left to right, the three columns represent the smooth case, a planet at 1 /3r_c, and a planet at 2/3r_c. From top to bottom, the rows represent three different snapshots at 300 kyr, 1 Myr, and 3 Myr. The white solid line is the SLR from Andrews et al. (2018b) and the red solid line our fit for the cases where a planet is included. The color bar shows the number of simulations in a single cell. The blue dash-dotted line shows the minimum limit (r_eff ~ 10 au) where observational results are available.