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Fig. A.2

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N2O profiles for planets around the Sun and M5V hosts at 100% and 1% PAL O2. The sun-hosted planet shows significant amounts of N2O depletion via photolysis (the main stratospheric sink of N2O), especially at lower O2 levels, as the UV protection from both O2 and O3 is significantly lessened. This depletion of N2O impacts the conversion of N2O to NOx. Meanwhile, the M5V-hosted planet experiences very little photolysis at all O2 levels, due to the low UV flux of the host star.

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