scCHIMERA radiative-convective-chemical equilibrium models where TiO and VO are assumed to have rained out of the atmosphere, along with the planet-to-star flux ratios from CHEOPS (orange), TESS (yellow), and Spitzer (black). The models are all for dayside-only redistribution (f=2) and varying metallicity. High albedo is obtained only at high metallicity through the condensation of MgSiO₃. The base of the silicate clouds is shown as a dot in the PT profile. When no dots are shown, the silicate does not form. Kzz was set to 10⁹ cm²/s and f_sed was set to 0.1, favoring small more reflective particles.