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Fig. B.1

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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 (KP ~ 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.

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