A homogeneous reanalysis of HARPS RVs for 87 small exoplanets provides RV amplitudes under 12 models and shows that eccentricity priors and GP activity modeling affect derived masses.
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Homogeneous planet masses I: Reanalysis of archival HARPS radial velocities
A homogeneous reanalysis of HARPS RVs for 87 small exoplanets provides RV amplitudes under 12 models and shows that eccentricity priors and GP activity modeling affect derived masses.