{
  "annotation_id": "4d5cc096-1934-4ea0-ae16-e4f0d52e0dd3",
  "date_created": "2026-03-02T18:00:43.530000Z",
  "date_modified": "2026-03-02T18:00:43.530000Z",
  "file_hash": "381ecd9c4d9ce9b9f770b0ab7a9c933f48d9b5e6c3b61eeae6f4241e7798857a",
  "private": false,
  "record": {
    "abstract": "Lobster-ISS is a revolutionary astrophysical X-ray all-sky monitor scheduled\nfor deployment as an attached payload on the International Space Station (ISS)\nin 2009. Using a new wide field-of-view focusing optic, Lobster-ISS provides an\norder-of-magnitude improvement in the sensitivity of all-sky monitors in the\nsoft X-ray band (0.1-3.0 keV). This lobster-eye optic presents unique\nchallenges to the imaging X-ray detector at its focus. Micro-patterned imaging\nproportional counters, with thier mechanical simplicity and high performance,\nare the most practical means of meeting the requirements. We describe our\ndesign for the Lobster-ISS imaging detector based on direct-imaging micro-well\nproportional counters and the expected performance.",
    "arxiv_id": "physics/0305025",
    "authors": [
      "J. K. Black",
      "A. N. Brunton",
      "N. P. Bannister",
      "P. Deines-Jones",
      "K. Jahoda"
    ],
    "categories": [
      "physics.ins-det",
      "astro-ph"
    ],
    "doi": "10.1016/j.nima.2003.08.015",
    "journal_ref": "Nucl.Instrum.Meth. A513 (2003) 123-126",
    "title": "The imaging X-ray detector for Lobster-ISS",
    "url": "https://arxiv.org/abs/physics/0305025"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "60f68445-3f13-4d29-b121-f5e36def1737",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}