Fig. 6

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Atmospheric chemical compositions after one year of simulation time for four atmospheres with water fractions of 100, 10, 1, and 0.1% arranged by columns, and four stellar forcing regimes arranged by rows: the YMDF, FF, FF400K, and CF models. Each panel shows the mixing ratios of key species after one year of chemical kinetic integration. In the constant flux regime it was allowed to the system to achieve a numerical steady state, if occurs before one year period. See supplementary animations online for 16 atmospheres under the YMDF model flaring.
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