Fig. 2
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Transmission spectrum of the hot Jupiter planet around a G2 star, for a Parker wind profile with Ṁ = 1010 g s−1 and T = 8000 K. The strongest line of each atomic and ionic species is marked if it exceeds our thresholds of 1% at λ < 4000 Å and 0.1% at λ > 4000 Å and its line-forming radius is shown in the top right panel of Fig. 3.
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