Corner plot showing the best-fit parameters for R_d, P, ω_l, and β to produce particle trajectories that match the projected distance and speed and periodicity of data from A. Boccaletti et al. (2018) (see, e.g., Figure 1). The prior bounds and best-fit values are shown in Table 1. The t_off parameter is not relevant for the actual simulations, but it helps find a better fit for the period of the planet. The remaining best-fit values are used for a large-scale simulation.