Fig. 4

Average transmission spectrum around the He I triplet in the planet rest-frame. The positions of the three helium lines are marked by vertical lines. The red curve is the best-fit Parker wind model obtained for a temperature of 6000 K and a mass-loss rate of 4.2 × 109 g s−1. The blue line indicates a model for a tentative blueward component centred at around −13 km s−1. The magenta dashed curve is the combination of the red and blue lines.
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