Fig. 7

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Distributions of orbital period, semimajor axis, minimum mass, eccentricity, and mass ratio q of M sin i > 40 MJup companions as obtained by the simultaneous radial velocity and proper motion anomaly fits for the 132 stars considered in Sect. 4. The minimum masses, eccentricity, and q distributions for inner (1 ≤ a < 5 au) and outer (a ≥ 5 au) companions found in the sample are shown in yellow and green, respectively.
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