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Fig. 4


Abundance weighted cross sections of relevant ions and molecules taken close to the 1.4 μm photosphere of WASP-121b (P = 40 mbar, T = 3100 K). The dashed line represents a scaled blackbody emission curve at a temperature of 3100 K (black, corresponding to the planet emission) and 6460 K (gray, corresponding to the incoming stellar light).

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