Fig. 11
Synthetic transmission spectra of GJ 436b’s atmosphere with a metallicity 100⊙. The different spectra correspond to the compositions at chemical equilibrium (green), and with disequilibrium compositions (Kzz = 109cm2 s−1) calculated with the Venot et al. (2012) scheme (blue), and with the updated scheme (red). The spectral resolving power is 300.
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