Cross-correlation matrices obtained by following the methods discussed in Sect. 2. Left column: Cross-correlation matrices in the Earth rest frame. The tilted dashed lines mark the exoplanet velocities. Right column: Cross-correlation matrices in the exoplanet rest-frame (K_P ~ 196 km s⁻¹). In this case, the exoplanet velocities are constantly 0 km s⁻¹ (vertical dashed lines). In all plots, the transit occurs between the horizontal dashed lines.