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Fig. A.1

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Chemical (coloured lines) and temperature (black dotted line) profiles derived from Exo-REM. The solid lines correspond to disequilibrium abundances and the dashed lines to chemical equilibrium abundances. The atmosphere is dominated by CH4 and not CO because of the low temperature. Although they are included in the computation, TiO and VO mixing ratios are negligible and do not appear on the plotted scale.

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