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Fig. A.1

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Nested-sampling posteriors retrieval from TauREx for the thermal inversion simulation considering TiO and VO as ab- sorbers in the atmosphere. We retrieved 12 free parameters, which are H2O, CO, TiO, and VO abundances in log10(VMR), the cloud pressure in Pa, four temperature points in Kelvin, two pressure points (in Pa), and the planetary radius in Jupiter’s radius. The molecular weight is derived from these parameters. T1 and T2 are the temperature points corresponding to the pressure points P1 and P2, respectively.

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