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Fig. 1
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Simulated outflow properties for the Neptune-like planet GJ 3470 b (Panel a) and for the hot Jupiter WASP-77A b (panel b). FXUV varies between 102 (deepest blue) and 106 erg cm−2 s−1 (deepest red), in intervals of 0.5 dex. The diamond symbols mark the location of the τ = 1 surface at 13.6 eV.
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