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Fig. 4

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HD 209458 b low-resolution ( ≈ 500) transit depth and species contributions simulated with Exo-REM. The grey areas represent the wavelength range of the CRIRES+ orders. On top are indicated the orders index number. From top to bottom: models with a C/O ratio of 0.1, 0.55, and 0.8, respectively. Dotted: the combined contributions of the H2−H2 and H2−He collision-induced absorptions and the effect of Rayleigh scattering. Dashed: the total contribution of the SiO2, Mg2SiO3 and Fe clouds for a cloud coverage of 1.0. The contributions of CO2, FeH, K, Na, PH3, TiO and VO were negligible in this spectral region and thus are not represented.

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