Total nucleation rate, J_* = ∑_i J_i [cm⁻³ s⁻¹], i = TiO₂, SiO, NaCl, KCl, in the 2D equatorial plane (θ = 0°) for the 1D profiles extracted from the 3D GCM models for log₁₀g = 3 [cgs]. The same cold model atmospheres similar to Fig. 2 are depicted. In this grid, the T_{eff, P} = 1400 K orbiting an K or G star is representative of NGTS-10b/WASP-43b and HD 209458b respectively. The T_{eff, P} = 1200 K orbiting the K dwarf may represent HD 189733b, T_{eff, P} = 1600 K orbiting the K star for WASP-63b.