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Fig. 4

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Retrieved best-fit pressure-temperature profiles when using GRAVITY (light blue) and all datasets except CRIRES+ (dark blue) for Exo-REM forward modeling. Shaded regions represent the 1 and 2 σ confidence interval, respectively. They are compared with the cloud optical depths of Mg2SiO4 (dashed brown) and Fe (dashed gray) defined as dτ = σc n dz with σc the effective extinction cross-section of the cloud (in m2), n its concentration (in particles/m3) and dz the thickness of the atmospheric layer (in m). The red curve represents the photosphere (region from which most thermal emission originates). In practice, we used a similar approach as Charnay et al. (2018) and constrained the pressure–temperature between the minimum and maximum of the brightness temperature computed between 0.625 to 10 µm.

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