Results of the cross-correlation analysis. Left column: synthetic model templates used for the individual molecules. Middle column: cross-correlation functions for every spectrum of all eight nights, sorted in phase and shifted to planet rest frame. The expected position of a signal should be vertical at v = 0 km s⁻¹ between the two horizontal dashed lines which indicate the first and last point of contact of the transit. Right column: K_p–v maps for each molecule. The expected position of a planetary signal is indicated by the dashed lines at K_p=102.5 km s⁻¹ and v = 0 km s⁻¹.