Cross-correlation values as a function of the orbital phase and planet orbital velocity in the Earth’s rest-frame. The results were obtained from 18 useful NIR orders. The orbital phase of the first and last in-transit spectra areindicated by horizontal dashed red lines. A visual guide to the expected exoplanet velocities (i.e., K_P = 140 km s⁻¹ and assuming no additional winds in the atmosphere of the planet) is indicated with tilted dashed red lines.