Fig. C.1

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Comparison of best-fit disequilibrium models to OSIRIS data from Ruffio et al. (2021). From top to bottom is HR 8799 b, c, and d. In blue are the best-fit disequilibrium models, with the spectra generated using high-resolution line-by-line opacities, before being convolved, binned, and normalised for comparison. In orange is the same, but with the metallicity set to 0.
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