and equilibrium gas-phase calculations like for HAT-P-7b (Sect 2.1 in [@2019arXiv190608127H]). In addition we include KCl as nucleation and growth species. The seed forming species need to be considered as surface growth material, too, since both processes (nucleation and growth) compete for the participating elements (Ti, Si, O, C, K, and Cl in this work). We consider the formation of 16 bulk materials (s=\[s\], \[s\], \[s\], MgO\[s\], SiO\[s\], \[s\], Fe\[s\], FeO\[s\], FeS\[s\], \[s\], \[s\], \[s\], \[s\], \[s\], C\[s\], KCl\[s\]; [ s indicating that this is a condensate material]{}) that form from 11 elements (Mg, Si, Ti, O, Fe, Al, Ca, S, C, K and Cl) by 128 surface reactions. The abundance of these 11 elements will decrease if cloud particles are forming (nucleation, growth) and increase if cloud particles evaporate. Sulfur has not been included in our present mineral cloud model. Sulfuric materials in form of S\[s\], FeS\[s\], MgS\[s\] would contribute by less than 10% in volume fraction in a solar element abundance gas [see Fig. 6 in @2019AREPS..47..583H].

[*Kinetic haze formation*]{}: We perform the simulations of photochemistry and haze formation using the models of [@2018ApJ...853....7K]. The procedure is the same as our previous studies [@2019ApJ...876L...5K; @2019ApJ...877..109K]: we first perform 