All the planetary systems simulated in this study are shown in the (Φ_p, F_XUV) plane, and color-coded based on the estimated mass loss rate illustrated by the right-hand side bar. Open, color-less circles show those cases for which ATES fails to converge. In general, known planets are identified by their names and highlighted by a circle; all the others are “synthetic”. ATES recovers stable, steady-state solutions for systems with log(−Φ_p)≲12.9 + 0.17 log F_XUV (in cgs units); such convergence threshold is marked by the dashed black line.