Fig. 14
Synthetic atmospheric spectra of TOI-776 b (red) and c (blue). Top: fiducial models with solar abundance (solid lines). Estimated uncertainties are shown for JWST NIRISS-SOSS, NIRSpec-G395M, and MIRI-LRS configurations, assuming two transits and binned for R = 50. Middle: enhanced carbon-to-oxygen ratio by a factor of two. Bottom: enhanced metallicity by a factor of 100. The left column represents spectra without haze opacity, and the right column with haze opacity.
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