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Fig. 9

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Atmospheric parameters for our equilibrium-chemistry models assuming solar abundances of heavy elements (solid), 50× solar (dashed), and 200× solar (dotted). The panels show as a function of altitude: a) the effective planetary radii, b) the temperature-pressure profiles, and c) the abundances of several molecular species. We discuss these models in Sect.4, and show the model transmission spectra derived from them in Fig. 8.

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