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Fig. A.2
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Abundances of O3 for both high CH4 models from this study and high N2O models from Kozakis et al. (2025) normalized to the amount of O3 with modern amounts of CH4 and N2O for all host stars at 0.1%, 1%, 10%, and 100% PAL O2. Both figures share the same color bar limits in order to facilitate comparisons.
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