Dynamical masses and improved orbits are determined for seven nearby star systems by jointly fitting thousands of radial velocities with Hipparcos and Gaia proper motion anomalies.
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The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems
Dynamical masses and improved orbits are determined for seven nearby star systems by jointly fitting thousands of radial velocities with Hipparcos and Gaia proper motion anomalies.