Comparison of azimuthally averaged radial profiles from the ¹²CO emission (in dotted red), dust continuum emission (in dashed gray), and gas density profile from each simulation setup (in solid blue), calculated as the median from the last 1000 orbits. The value of a_bin is calculated for each simulation to match the peak density position with the peak brightness position of the dust continuum. The values for e_bin increase from left to right, and each row has a constant disk aspect ratio. The average radial resolution of the ¹²CO and dust continuum are shown in the upper left panel, with Gaussians of the same colors. A dashed vertical line marks the position of the simulated planet.