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Fig. 4

image

Simulated transmission spectrum of the medium CH4 scenario with the H2-dominated atmosphere (scenario 1b) binned to a constant resolving power of R = 300 (maximum resolving power of JWST NIRSpec PRISM at 5 μm). The black line represents the spectrum that includes the contribution from all gases which are considered in 1D-TERRA and also available in HITRAN, Rayleigh scattering, aerosol extinction, H2O CKD, and CIAs. Individual gaseous absorption of selected molecules are represented by different colors.

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