Radial velocity comparison of Gaia DR2 and RAVE DR5 survey: a systematic offset in radial velocities among a group of highly accurate radial velocity stars
arXiv:1807.11716 · doi:10.3847/1538-3881/aadcde
Abstract
Here, we report comparative study of radial velocity () data of two major surveys: Gaia Data Release 2 and RAVE Data Release 5. We restricted the sample to stars with relatively accurate radial velocities ( 2 km s or 2%, and 2 km s or 2%). The difference between and for a majority of the sample follows normal distribution with mean = 0.28 km s and = 1.49 km s. However, we found a very small group of stars ( of the total) for which the difference in radial velocities between the two surveys is significantly larger with an offset of 104.50 km s with = 4.92 km s. Kinematics based on 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 radial velocity is probably due to RAVE velocity data for this particular group.
7 pages, 6 figures, accepted for publication in the Astronomical Journal on July 25, 2018
References in corpus (5)
Cited by in corpus (4)
- APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South
- Gaia Data Release 3: Mapping the asymmetric disc of the Milky Way
- Survey of Surveys I: The largest catalogue of radial velocities for the Galaxy
- Gaia Early Data Release 3: Updated radial velocities from Gaia DR2