Spectroscopic and photometric data for likely member stars of five Galactic globular clusters (M3, M53, M71, M92, and NGC 5053) and three open clusters (M35, NGC 2158, and NGC 6791) are processed by the current version of the SEGUE Stellar Parameter Pipeline (SSPP), in order to determine estimates of metallicities and radial velocities (RVs) for the clusters. These results are then compared to values from the literature.
Cone search capability for table J/AJ/141/89/table1 (Literature properties of globular and open clusters)
Cone search capability for table J/AJ/141/89/table4 (Properties of adopted true member stars)