Atmospheric mass-loss rates predicted by the hydrodynamic model for planets with R_pl = 5 R_⊕ and M_pl between 1 M_⊕ and 108.6 M_⊕ orbiting a 0.6 M_⊙ star at an orbital separation corresponding to T_eq values of 300K (blue circles), 700K (green circles), 1100 K (deep yellow circles), 1500 K (violet circles), and 2000 K (red circles) as a function of M_pl (top), Λ (middle), and Λ × K (bottom). Lines of different styles indicate the mass-loss rates predicted by the energy-limited approximation Ṁ_EL (dash-dotted), core-powered mass loss Ṁ_CP (solid), and Roche lobe overflow Ṁ_RL (dashed), with the colour of the lines following the same scheme as that of the circles. For Ṁ_EL, we considered the same EUV fluxes as for the hydrodynamic models shown in the plots, namely 3.0 erg s cm⁻² for the orbital separation corresponding to T_eq of 300 K, 89.1 erg s cm⁻² for 700K, 543.3 erg scm⁻² for 1100K, 1878.6 ergs cm⁻² for 1500 K, and 5937.3 erg s cm⁻² for 2000 K.