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Fig. 1

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Rossiter-McLaughlin effect as seen from HARPS RVs centred around the mid-transit time after subtracting the Keplerian motion induced by the planet. The grey line shows the RM effect with the best-fitting (retrograde) model as the solid line and an aligned model as the dashed line. The error bars include the jitter term from our MCMC added in quadrature, shown as the black extension.

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