Fig. B.1
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Accuracy validation of reduced FastChem input compared to the complete, extended equilibrium-chemistry model. Left panels : deviation in VMRs for a solar composition (Asplund et al. 2021), a 10 times solar metallicity, and a C/O = 1.0, assuming a Teff = 1300 K temperature profile (Mukherjee et al. 2024). Right panels : RMSE between the log VMRs of the two inputs at varying metallicities and C/O ratios.
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