Fig. 11
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Synthetic transmission spectrum model of TOI-674b (gray line) in the JWST spectral range computed with petitRADTRANS (Mollière et al. 2019). The model assumes solar abundance and a cloud-free atmosphere with an isothermal temperature of 700 K. PandExo (Batalha et al. 2017) simulations of TOI-674b transmission spectrum observationsmade with JWST instruments NIRISS (blue), NIRSpec (orange), and MIRI (red) are also shown.
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