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Fig. 10

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Transmission spectroscopy near the He I triplet. Panels a and b show the 2D transmission spectroscopy maps in the stellar and planet rest frames, respectively. Tilted and vertical lines denote the position of the He I triplet, while horizontal dotted lines mark the transit contact points, t1, t2, t3, and t4. Panel c shows the spectroscopic light curve computed in a 0.075 nm band centred around the peak of absorption. Vertical dashed lines mark the transit contact points. Panel d presents the full in-transit averaged transmission spectrum.

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