Fig. C.1.
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Spectrum from the MIRI LRS Eureka! data reduction (Luque et al. 2025) (error bars) compared to the best nonequilibrium model from Jaziri et al. (2025) (solid black line) fitting the NIRISS SOSS/NIRSpec G395H observations. The spectrum is also compared to the two MIRI LRS nonequilibrium retrieval solutions (solid light black line: low metallicity; solid blue line: high metallicity) and to the best MIRI LRS model (solid light blue line), all shown at a resolution of 200. Key spectral features are highlighted in the corresponding colors.
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