Fig. 20
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Synthetic transit spectra of GJ 3090 b. The estimated uncertainties are calculated with the JWST ETC PandExo (Batalha et al. 2017) using NIRISS (SOSS; blue) with the NIRSPec (395M grism; green) and with MIRI (LRS; red) instrument modes of the JWST. This calculation assumes a 1000x solar metallicity atmosphere (with a cloud top at 1 millibar). The initial modelled transit spectrum is plotted in grey.
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