The APO-K2 Catalog. I. ~7,500 Red Giants with Fundamental Stellar Parameters from APOGEE DR17 Spectroscopy and K2-GAP Asteroseismology
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Schonhut-Stasik, Jessica1
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Zinn, Joel2
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Stassun, Keivan, G.1
- Pinsonneault, Marc3
- Johnson, Jennifer4
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Warfield, Jack5
- Stello, Dennis6
- Elsworth, Yvonne7
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García, Rafael, A.8
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Mathur, Savita9
- Mosser, Benoit10
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Marc Hon11
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Tayar, Jamie12
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Stringfellow, Guy, S.13
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Beaton, Rachael, L.14
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Jönsson, Henrik15
- Minniti, Dante16
- 1. Vanderbilt University, TN
- 2. California State University (Long Beach), CA
- 3. The Ohio State University, OH
- 4. The Ohio State University, OH
- 5. The University of Virginia, VA
- 6. University of New South Wales, Australia
- 7. Aarhus University, Denmark
- 8. Université Paris Cité, France
- 9. Instituto de Astrofísica de Canarias, Tenerife
- 10. Université de Paris, France
- 11. University of Hawai'i (at Manoa)
- 12. University of Florida, FL
- 13. University of Colorado at Boulder, CO
- 14. Space Telescope Science Institute, MD
- 15. Malmö University, Sweden
- 16. Universidade Federal de Santa Catarina, Brazil
Description
Abstract: We present a catalog of fundamental stellar properties for ~7,500 evolved stars, including stellar radii and masses, determined from the combination of spectroscopic observations from the Apache Point Observatory Galactic Evolution Experiment (APOGEE), part of the Sloan Digital Sky Survey IV (SDSS), and asteroseismology from K2. The resulting APO-K2 catalog provides spectroscopically derived temperatures and metallicities, asteroseismic global parameters, evolutionary states, and asteroseismically-derived masses and radii. Additionally, we include kinematic information from Gaia. We investigate the multi-dimensional space of abundance, stellar mass, and velocity with an eye toward applications in Galactic archaeology. The APO-K2 sample has a large population of low metallicity stars (~288 at [M/H] ≤ -1), and their asteroseismic masses are larger than astrophysical estimates. We argue that this may reflect offsets in the adopted fundamental temperature scale for metal-poor stars rather than metallicity-dependent issues with interpreting asteroseismic data. We characterize the kinematic properties of the population as a function of α-enhancement and position in the disk and identify those stars in the sample that are candidate components of the Gaia-Enceladus merger. Importantly, we characterize the selection function for the APO-K2 sample as a function of metallicity, radius, mass, νmax, color, and magnitude referencing Galactic simulations and target selection criteria to enable robust statistical inferences with the catalog.
Included Files:
- The publicly available APO-K2 catalog, the is provided in the publication.
- The APO-K2 catalog without truncation to any numbers.
- The selection function relative density tables for the mass-radius parameter space.
- The selection function relative density tables for the metallicity-mass parameter space.
- The selection function relative density tables for the magnitude-color parameter space.
- The selection function relative density tables for the νmax-mag parameter space.
Files
apo_k2_public_catalog.csv
Files
(9.9 MB)
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Additional details
Related works
- Is derived from
- Dataset: https://github.com/Jesstella/APO-K2 (URL)
- Is supplement to
- Preprint: https://arxiv.org/abs/2304.10654 (URL)
- Other: https://www.jessicastasik.com/apo-k2 (URL)