Reflected light models of WASP-80 b for a variety of cloud species produced with PICASO and VIRGA, considering a Bond albedo of 0.25. The full and dashed lines correspond to models with sedimentation efficiencies f_sed of 0.1 and 3, respectively. The models are compared to our measured secondary eclipse spectrum (black and white points, binned by a factor of 2) for wavelengths below 1.6 μm, where the contribution from thermal emission is minimal, as shown by the pink dotted line. The short-wavelength spectrum is best explained by either chromium (Cr), intermediate-sedimentation sodium sulfide (Na₂S), potassium chloride (KCl), or low-sedimentation zinc sulfide (ZnS) clouds.