{
  "annotation_id": "a703acc5-0bd5-4988-9546-34c4c0df0121",
  "date_created": "2026-03-02T18:01:11.528000Z",
  "date_modified": "2026-03-02T18:01:11.528000Z",
  "file_hash": "645c32bc6d579b114b1d24b64d26e53609f33334c3bb0a45f6aa702a73c6ee29",
  "private": false,
  "record": {
    "abstract": "Scintillation light from gamma ray irradiation in liquid xenon is detected by\ntwo Hamamatsu R9288 photomultiplier tubes (PMTs) immersed in the liquid. UV\nlight reflector material, PTFE, is used to optimize the light collection\nefficiency. The detector gives a high light yield of 6 photoelectron per keV\n(pe/keV), which allows efficient detection of the 122 keV gamma-ray line from\nCo-57, with a measured energy resolution of (8.8+/-0.6)% (sigma). The best\nachievable energy resolution, by removing the instrumental fluctuations, from\nliquid xenon scintillation light is estimated to be around 6-8% (sigma) for\ngamma-ray with energy between 662 keV and 122 keV.",
    "arxiv_id": "physics/0608034",
    "authors": [
      "K. Ni",
      "E. Aprile",
      "K. L. Giboni",
      "P. Majewski",
      "M. Yamashita"
    ],
    "categories": [
      "physics.ins-det",
      "astro-ph",
      "nucl-ex"
    ],
    "doi": "10.1088/1748-0221/1/09/P09004",
    "journal_ref": "JINST1:P09004,2006",
    "title": "Gamma Ray Spectroscopy with Scintillation Light in Liquid Xenon",
    "url": "https://arxiv.org/abs/physics/0608034"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "592ddcfa-8679-4ba3-9822-5d0b910e9636",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}