Abstract
Abstract Here, we report a comparative study of radial velocity (RV) data of two major surveys: Gaia Data Release 2 and RAVE Data Release 5. We restricted the sample to stars with relatively accurate RVs ( km s−1 or ≤2%, and km s−1 or ≤2%). The difference between RV Gaia and RVRAVE for a majority of the sample follows a normal distribution with mean = 0.28 km s−1 and σ = 1.49 km s−1. However, we found a very small group of stars (≈0.08% of the total) for which the difference in RVs between the two surveys is significantly larger with an offset of −104.50 km s−1 with σ = 4.92 km s−1. Kinematics based on RV Gaia suggest that most of the group members belong to the Galactic thin disk, which agrees with the group’s metallicity range of −1.2 to +0.5 dex suggesting the offset in RV is probably due to RAVE velocity data for this particular group.
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