Fig. 15
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Synthetic JWST transmission atmospheric spectra of TOI-1468 b and c. Fiducial models with solar abundances and no haze (solid blue and red lines), with haze (dodger blue and orange), and enhanced metallicity by a factor of 100 (cyan and gold). Estimated uncertainties are shown for the simulated observation of one transit with JWST NIRISS-SOSS, NIRSpec-G395M, and MIRI-LRS configurations.
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