Fig. A.1
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Transmission spectra shown in tomography in the planetary rest frame for the three consideredtransits, as a function of wavelength and planetary orbital phase. The contact points t1, t2, t3, and t4 are marked with horizontal black lines. The feature at 1083.5 nm misaligned with theplanet rest frame present on the first and second night is a residual of a telluric H2O line.
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