{
  "annotation_id": "58a1214e-8a97-467e-9c77-d1d2d8d27f13",
  "date_created": "2026-03-02T18:00:53.857000Z",
  "date_modified": "2026-03-02T18:00:53.857000Z",
  "file_hash": "1161eae8cc9410362825b5996bc4acb262a13b91753e607721e7d538c44fa806",
  "private": false,
  "record": {
    "abstract": "Three slow glitches in the rotation rate of the pulsar B1822-09 were revealed\nover the 1995-2004 interval. The slow glitches observed are characterized by a\ngradual increase in the rotation frequency with a long timescale of several\nmonths, accompanied by a rapid decrease in the magnitude of the frequency first\nderivative by 1-2 per cent of the initial value and subsequent exponential\nincrease back to its initial value on the same timescale. The cumulative\nfractional increase in the pulsar rotation rate for the three glitches amounts\nto Delta_nu/nu ~ 7 10^{-8}.",
    "arxiv_id": "physics/0411151",
    "authors": [
      "T. V. Shabanova"
    ],
    "categories": [
      "physics.data-an",
      "astro-ph"
    ],
    "doi": "10.1111/j.1365-2966.2004.08580.x",
    "journal_ref": "Mon.Not.Roy.Astron.Soc. 356 (2005) 1435-1439",
    "title": "Observations of three slow glitches in the spin rate of the pulsar   B1822-09",
    "url": "https://arxiv.org/abs/physics/0411151"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "0319e802-2b0b-483b-bc5c-e081f61089a5",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}