{
  "id": "1309.4733",
  "version": "v1",
  "published": "2013-09-18T18:13:50.000Z",
  "updated": "2013-09-18T18:13:50.000Z",
  "title": "Infrared Laboratory Oscillator Strengths of Fe I in the H-Band",
  "authors": [
    "M. P. Ruffoni",
    "J. C. Pickering",
    "C. Allende Prieto",
    "G. Nave"
  ],
  "comment": "To appear in the Astrophysical Journal",
  "categories": [
    "astro-ph.SR",
    "astro-ph.IM"
  ],
  "abstract": "We report experimental oscillator strengths for 28 infrared Fe I transitions, for which no previous experimental values exist. These transitions were selected to address an urgent need for oscillator strengths of lines in the H-band (between 1.4 um and 1.7 um) required for the analysis of spectra obtained from the Sloan Digital Sky Survey (SDSS-III) Apache Point Galactic Evolution Experiment (APOGEE). Upper limits have been placed on the oscillator strengths of an additional 7 transitions, predicted to be significant by published semi-empirical calculations, but not observed to be so.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2013-09-18T18:13:50.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "infrared laboratory oscillator strengths",
      "apache point galactic evolution experiment",
      "report experimental oscillator strengths",
      "sloan digital sky survey"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1088/0004-637X/779/1/17",
      "journal": "The Astrophysical Journal",
      "year": 2013,
      "month": "Dec",
      "volume": 779,
      "number": 1,
      "pages": 17
    },
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1254551,
      "adsabs": "2013ApJ...779...17R"
    }
  }
}