{
  "id": "1308.1332",
  "version": "v1",
  "published": "2013-08-06T16:26:36.000Z",
  "updated": "2013-08-06T16:26:36.000Z",
  "title": "Infrared composition of the Large Magellanic Cloud",
  "authors": [
    "M. Siudek",
    "A. Pollo",
    "T. T. Takeuchi",
    "Y. Ita",
    "D. Kato",
    "T. Onaka"
  ],
  "journal": "Earth Planets Space, Vol. 65 (No. 3), pp. 229-271, 2013",
  "doi": "10.5047/eps.2012.09.001",
  "categories": [
    "astro-ph.GA",
    "astro-ph.CO"
  ],
  "abstract": "The evolution of galaxies and the history of star formation in the Universe are among the most important topics in today's astrophysics. Especially, the role of small, irregular galaxies in the star-formation history of the Universe is not yet clear. Using the data from the AKARI IRC survey of the Large Magellanic Cloud at 3.2, 7, 11, 15, and 24 {\\mu}m wavelengths, i.e., at the mid- and near-infrared, we have constructed a multiwavelength catalog containing data from a cross-correlation with a number of other databases at different wavelengths. We present the separation of different classes of stars in the LMC in color-color, and color-magnitude, diagrams, and analyze their contribution to the total LMC flux, related to point sources at different infrared wavelengths.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2013-08-06T16:26:36.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "large magellanic cloud",
      "infrared composition",
      "akari irc survey",
      "total lmc flux",
      "multiwavelength catalog containing data"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "journal": "Earth, Planets, and Space",
      "year": 2013,
      "month": "Mar",
      "volume": 65,
      "number": 3,
      "pages": 229
    },
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1246757,
      "adsabs": "2013EP&S...65..229S"
    }
  }
}