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Target Selection for the SDSS-IV APOGEE-2 Survey

Journal Article · · Astronomical Journal (Online)
 [1]; ; ;  [2]; ;  [3];  [4]; ;  [5];  [6];  [7]; ;  [8];  [9];  [10]; ;  [11];  [12];  [13];
  1. Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 (United States)
  2. Space Telescope Science Institute, Baltimore, MD 21218 (United States)
  3. Department of Astronomy, New Mexico State University, Las Cruces, NM 88001 (United States)
  4. Departamento de Astronomía, Universidad de Chile, Santiago (Chile)
  5. Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235 (United States)
  6. PITT PACC, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260 (United States)
  7. The Observatories of the Carnegie Institution for Science, Pasadena, CA 91101 (United States)
  8. Steward Observatory, The University of Arizona, Tucson, AZ 85719 (United States)
  9. Department of Astronomy and Astrophysics and Dunlap Institute for Astronomy and Astrophysics, University of Toronto, Toronto, ON M5S 3H4 (Canada)
  10. Department of Physics and Astronomy, Western Washington University, Bellingham, WA 98225 (United States)
  11. Departamento de Astrofísica, Universidad de La Laguna, and Instituto de Astrofísica de Canarias, La Laguna, Tenerife (Spain)
  12. Department of Physics and Astronomy, Texas Christian University, Fort Worth, TX 76129 (United States)
  13. Department of Astronomy, Case Western Reserve University, Cleveland, OH 44106 (United States)
APOGEE-2 is a high-resolution, near-infrared spectroscopic survey observing ∼3 × 10{sup 5} stars across the entire sky. It is the successor to APOGEE and is part of the Sloan Digital Sky Survey IV (SDSS-IV). APOGEE-2 is expanding on APOGEE’s goals of addressing critical questions of stellar astrophysics, stellar populations, and Galactic chemodynamical evolution using (1) an enhanced set of target types and (2) a second spectrograph at Las Campanas Observatory in Chile. APOGEE-2 is targeting red giant branch and red clump stars, RR Lyrae, low-mass dwarf stars, young stellar objects, and numerous other Milky Way and Local Group sources across the entire sky from both hemispheres. In this paper, we describe the APOGEE-2 observational design, target selection catalogs and algorithms, and the targeting-related documentation included in the SDSS data releases.
OSTI ID:
22663121
Journal Information:
Astronomical Journal (Online), Journal Name: Astronomical Journal (Online) Journal Issue: 5 Vol. 154; ISSN 1538-3881
Country of Publication:
United States
Language:
English