Published February 3, 2022 | Version v1
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Spectro-photometric distances and self-calibrated abundances for Apogee DR16 RGB stars within the Milky Way disk

  • 1. MIT
  • 2. Flatiron Institute
  • 3. MPIA
  • 4. Columbia University
  • 5. Gothard Astrophysical Observatory
  • 6. Universidad de Antofagasta

Description

The data file contains 48,853 RGB stars from Apogee DR16 within the Milky Way disk, for which we determine spectro-photometric parallax estimates (as described in Hogg et al. 2019, AJ, 158, 147), as well as self-calibrated stellar element abundances. The data set is described in detail and analyzed in Eilers et al. 2022 (arXiv: 2112.03295).

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