{
  "id": "astro-ph/0009369",
  "version": "v1",
  "published": "2000-09-22T15:31:56.000Z",
  "updated": "2000-09-22T15:31:56.000Z",
  "title": "High Energy Gamma Rays",
  "authors": [
    "R. Mukherjee"
  ],
  "comment": "7 pages, 5 figures. Invited lecture at the Neutrino 2000 conference, Sudbury, Canada",
  "journal": "Nucl.Phys.Proc.Suppl.91:480-486,2001",
  "doi": "10.1016/S0920-5632(00)00978-6",
  "categories": [
    "astro-ph"
  ],
  "abstract": "This article reviews the present status of high energy gamma-ray astronomy at energies above 30 MeV. Observations in the past decade using both space- and ground-based experiments have been primarily responsible for giving a tremendous boost to our knowledge of the high energy Universe. High energy gamma-rays have been detected from a wide range of Galactic and extragalactic astrophysical sources, such as gamma-ray bursters, pulsars, and active galaxies. These observations have established high energy gamma-ray astronomy as a vital and exciting field, that has a bright future. This review summarizes the experimental techniques, observations and results obtained with recent experiments, and concludes with a short description of future prospects.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2000-09-22T15:31:56.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "high energy gamma rays",
      "established high energy gamma-ray astronomy",
      "observations",
      "high energy universe",
      "past decade"
    ],
    "tags": [
      "conference paper",
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 7,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 534083
    }
  }
}