{
  "id": "1409.2277",
  "version": "v1",
  "published": "2014-09-08T10:39:26.000Z",
  "updated": "2014-09-08T10:39:26.000Z",
  "title": "Early Results from APOKASC",
  "authors": [
    "Courtney Epstein"
  ],
  "comment": "Proc. of the workshop \"Asteroseismology of stellar populations in the Milky Way\" (Sesto, 22-26 July 2013), Astrophysics and Space Science Proceedings, (eds. A. Miglio, L. Girardi, P. Eggenberger, J. Montalban)",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "Asteroseismology and spectroscopy provide complementary constraints on the fundamental and chemical properties of stars. I describe the first results from APOKASC, a collaboration between the Kepler asteroseismic science consortium (KASC) and the SDSS-III APOGEE survey. These include (1) the first test of asteroseismic scaling relationships in the metal-poor regime using halo and thick disk stars identified in the APOKASC sample; and (2) the calibration of spectroscopic parameters using precise asteroseismic measurements of surface gravity. I also highlight future research avenues that are made possible by this unique sample of thousands of well-characterized red giant stars.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2014-09-08T10:39:26.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "early results",
      "kepler asteroseismic science consortium",
      "precise asteroseismic measurements",
      "sdss-iii apogee survey",
      "thick disk stars"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1007/978-3-319-10993-0_15",
      "journal": "Astrophysics and Space Science Proceedings",
      "year": 2015,
      "volume": 39,
      "pages": 133
    },
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "adsabs": "2015ASSP...39..133E"
    }
  }
}