Condensation sequences of all possible solid species (Table 2) in the equilibrium condensation simulations for Kepler-94 (the most metalrich) and Kepler-62 (the most metal-poor) stars computed using ECCOplanets code (Timmermann et al. 2023). The molar amount relative to the total molar content in the disk for each of the condensates is displayed as a function of decreasing disk temperature at a constant disk pressure of 4.2 × 10⁻⁴ bar. Stellar abundances are from Brewer et al. (2016), with S abundances estimated based on [Fe/H] values.