Planetary radius (top) and mass-loss rate (bottom) evolutionary tracks for planets 16 (left; M_* =0.7 M_⊙; T_eq = 1700K; a = 0.0113 AU; $M_{\text{pl}}^0=30M_{\oplus }$; $f_{\text{at}}^0=0.090$), 22 (center; M_* = 0.5 M_⊙; T_eq = 1000 K; a = 0.0151 AU; $M_{\text{pl}}^0=9M_{\oplus }$; $f_{\text{at}}^0=0.050$), and 25 (right; ; M_* = 0.5 M_⊙; T_eq = 1000K; a = 0.0151 AU; $M_{\text{pl}}^0=17M_{\oplus }$; $f_{\text{at}}^0=0.196$; see Table 2), as predicted employing MLink (blue lines), interpol2024 (red lines), energy-limited approximation (black lines), and core-powered mass loss (green lines), or the combination of the latter two (cyan).