Fig. D.2
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Left: Simulated spectra of TOI-5789 at Ariel’s Tier-3 resolution, assuming 1× (blue) and 100× (orange) solar metallicities. The lower part of the panel shows the scaled contributions of different molecules. Right: Retrieved chemical abundances. The dashed vertical lines indicate the true values for each species, while the colored regions of the histograms represent the 15.86%-84.14% quantiles of the posterior distributions.
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