Fig. 12
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Condensation curves of several potential cloud-forming species (thin coloured lines) overplotted on the P−T profile from the radiative-convective equilibrium model (thick blue line). The condensation curves assume a gas with 10× solar metallicity. The shaded areas are the cloud pressure one-sigma ranges derived from the retrievals using the TEATRO reduction (pink) and the CASCADe reduction (blue).
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