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Title: THE SEGUE STELLAR PARAMETER PIPELINE. IV. VALIDATION WITH AN EXTENDED SAMPLE OF GALACTIC GLOBULAR AND OPEN CLUSTERS

Journal Article · · Astronomical Journal (New York, N.Y. Online)
; ;  [1];  [2]; ;  [3];  [4];  [5];  [6];  [7]
  1. Department of Physics and Astronomy and JINA (Joint Institute for Nuclear Astrophysics), Michigan State University, East Lansing, MI 48824 (United States)
  2. Department of Science Education, Ewha Womans University, Seoul 120-750 (Korea, Republic of)
  3. Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States)
  4. Department of Astronomy, Ohio State University, 140 West 18th Avenue, Columbus, OH 43210 (United States)
  5. UCO/Lick Observatory, University of California, Santa Cruz, CA 95064 (United States)
  6. IIAP: Indian Institute of Astrophysics, II Block, Koramangala, Bangalore 560 034 (India)
  7. Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States)

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. We find that the mean metallicity (([Fe/H])) and mean radial velocity ((RV)) estimates for each cluster are almost all within 2{sigma} of the adopted literature values; most are within 1{sigma}. We also demonstrate that the new version of the SSPP achieves small, but noteworthy, improvements in ([Fe/H]) estimates at the extrema of the cluster metallicity range, as compared to a previous version of the pipeline software. These results provide additional confidence in the application of the SSPP for studies of the abundances and kinematics of stellar populations in the Galaxy.

OSTI ID:
21583203
Journal Information:
Astronomical Journal (New York, N.Y. Online), Vol. 141, Issue 3; Other Information: DOI: 10.1088/0004-6256/141/3/89; ISSN 1538-3881
Country of Publication:
United States
Language:
English