Detectability of biosignatures in warm, water-rich atmospheres

Open Access

Fig. A.1

Individual VMRs of H (a), OH (b), and HO₂ (c) that summed together produce the profile of the HO_X chemical group (Figure 3b), as well as H₂O₂ (d), a reservoir for HO_X species, for biotic model runs at solar constant 1.0, 1.1, 1.2, 1.3, 1.4, and 1.5 (see Figure 1 for the colour legend).

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