{
  "annotation_id": "ab88958a-194f-49bc-b950-d4ae1ce70141",
  "date_created": "2026-03-02T18:01:18.446000Z",
  "date_modified": "2026-03-02T18:01:18.446000Z",
  "file_hash": "6337018804c41b2470635232f24b86ec3636921e9240b8770e31a7ee8bafdc2b",
  "private": false,
  "record": {
    "abstract": "LXeGRIT - Liquid Xenon Gamma-Ray Imaging Telescope - is the first prototype\nof a Compton telescope for \\MeV \\g-ray astrophysics based on a LXe time\nprojection chamber. One of the most relevant figures of merit for a Compton\ntelescope is the detection efficiency for \\g-rays, which depends on diverse\ncontributions such as detector geometry and passive materials, trigger\nefficiency, dead time, etc. A detailed study of the efficiency of the LXeGRIT\ninstrument, based both on laboratory measurements and Monte Carlo simulations,\nis presented in this paper.",
    "arxiv_id": "physics/0702078",
    "authors": [
      "A. Curioni",
      "E. Aprile",
      "T. Doke",
      "K. L. Giboni",
      "M. Kobayashi",
      "U. G. Oberlack"
    ],
    "categories": [
      "physics.ins-det",
      "astro-ph"
    ],
    "doi": "10.1016/j.nima.2007.02.102",
    "journal_ref": "Nucl.Instrum.Meth.A576:350-361,2007",
    "title": "A Study of the LXeGRIT Detection Efficiency for MeV Gamma-Rays during   the 2000 Balloon Flight Campaign",
    "url": "https://arxiv.org/abs/physics/0702078"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "6de7f922-181b-4d2b-9dde-64ee0d48357c",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}