{
  "id": "1610.08061",
  "version": "v1",
  "published": "2016-10-25T20:00:07.000Z",
  "updated": "2016-10-25T20:00:07.000Z",
  "title": "A new catalog of homogenised absorption line indices for Milky Way globular clusters from high-resolution integrated spectroscopy",
  "authors": [
    "Hak-Sub Kim",
    "Jaeil Cho",
    "Ray M. Sharples",
    "Alexandre Vazdekis",
    "Michael A. Beasley",
    "Suk-Jin Yoon"
  ],
  "comment": "21 pages, 10 figures, accepted for publication in ApJS",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "We perform integrated spectroscopy of 24 Galactic globular clusters. Spectra are observed from one core radius for each cluster with a high wavelength resolution of ~2.0 A FWHM. In combination with two existing data sets from Puzia et al. (2002) and Schiavon et al. (2005), we construct a large database of Lick spectral indices for a total of 53 Galactic globular clusters with a wide range of metallicities, -2.4 < [Fe/H] < 0.1, and various horizontal-branch morphologies. The empirical index-to-metallicity conversion relationships are provided for the 20 Lick indices for the use of deriving metallicities for remote, unresolved stellar systems.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2016-10-25T20:00:07.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "milky way globular clusters",
      "homogenised absorption line indices",
      "high-resolution integrated spectroscopy",
      "galactic globular clusters"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 21,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}