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Fig. A.1

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Correction of the residual of the planetary obscuration of the stellar disc (Doppler shadow). The planetary trace is shown in white. The dashed black lines indicate the start and the end of the transit. Top panel: Two-dimensional cross-correlation function. Middle panel: Model of the residual of the planetary obscuration of the stellar disc with two Gaussian components. Bottom panel: Two-dimensional cross-correlation function after correction.

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