Fig. 5
Comparison between the HST/WFC3 dataset of Spake et al. (2018) in blue with our degraded high-resolution CARMENES dataset in red. Transmission spectra are binned over 98 Å. Lighter points correspond to the same transmisssion spectra, but shifted by 24.5, 49.0, and 73.5 Å. The vertical grey dashed line is the helium triplet transition.
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