Fig. G.2.
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Left: CCF of the Ti+ mask with the retrieved planetary spectrum for WASP-121b (night 2, 4UTs). Center: CCF built from considering the contributions from spectra between -15 km/s and 15 km/s in the stellar frame of reference alone. Right: Same as the initial CCF, but excluding the previous stellar contribution region. All the plots are in the planetary rest frame.
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