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Fig. 1
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CORALIE radial velocity measurements of MASCARA-4, phase folded on the planetary orbital period and corrected for steller activity. The best-fit Keplerian model to the data is shown as a solid grey line. The semi-amplitude of the stellar reflex motion is 165.9 ± 23.7m s−1, corresponding to aplanetmass of 1.675 ± 0.241 MJup.
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