Development of a C/H/O/N/S chemical network: Experimental benchmark, application to exoplanets, and identification of key C/S coupling pathways

Open Access

Fig. 3

Abundance profiles of GJ 436 b, GJ 1214 b, HD 189733 b, HD 209458 b, WASP-39 b, and WASP-107 b simulated with FRECKLL. Solid lines show results from the present work, while dashed lines show those from Tsai 2023. We omit H₂ and He for clarity to focus on the main species.

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