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Fig. 3

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Calculated dayside composition in five gas giants and three plausible secondary atmospheres (hot volcano-like, hot reducing N2/CH4, and warm oxidizing N2/O2 atmosphere). Dotted lines correspond to the initial composition (chemical equilibrium for the gas giants and equal uniform abundances for secondary atmospheres), dashed lines to a calculation where the initial temperature does not further evolve (only for the gas giants), and solid lines to a self-consistent calculation where temperature and chemical composition evolve together.

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