Fig. A.1
Atmospheric composition profiles used for radiative transfer in the LMDG GCM and for 1×, 10×, 100×, 300×, and 1000× solar metallicity. Chemical abundances are computed with Exo-REM with non-equilibrium chemistry for an eddy-mixing coefficient Kzz=106 cm2 s−1 and for solar C/O ratio. We note that the mixing ratio of water is computed separately in the GCM with cloud condensation.
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