Fig. 2
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Top: telluric transmission as a function of wavelength obtained from ESO SkyCalc (Noll et al. 2012). Middle: transit depth as a function of wavelength, modelled using petitRADTRANS over the entire CARMENES NIR channel and assuming an isothermal atmosphere at the planet equilibrium temperature of 2160 K. The red region indicates the spectral range used for our analysis. Bottom: same but for T = 3200 K.
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