{
  "annotation_id": "e2ec9d9a-4a54-4c8c-9093-62c00fbc5252",
  "date_created": "2026-03-02T18:00:39.110000Z",
  "date_modified": "2026-03-02T18:00:39.110000Z",
  "file_hash": "afe2c15a810fbde72211d3c49bf50879993822b0b2c18c733f8025e40e754bb7",
  "private": false,
  "record": {
    "abstract": "A system based on ROOT for handling the micro-DST of the BaBar experiment is\ndescribed. The purpose of the Kanga system is to have micro-DST data available\nin a format well suited for data distribution within a world-wide collaboration\nwith many small sites. The design requirements, implementation and experience\nin practice after three years of data taking by the BaBar experiment are\npresented.",
    "arxiv_id": "physics/0206067",
    "authors": [
      "T. J. Adye",
      "A. Dorigo",
      "R. Dubitzky",
      "A. Forti",
      "S. J. Gowdy",
      "G. Hamel de Monchenault",
      "R. G. Jacobsen",
      "D. Kirkby",
      "S. Kluth",
      "E. Leonardi",
      "A. Salnikov",
      "L. Wilden"
    ],
    "categories": [
      "physics.comp-ph"
    ],
    "doi": "10.1016/S0010-4655(02)00678-1",
    "journal_ref": "Comput.Phys.Commun.150:197-214,2003",
    "title": "KANGA(ROO): Handling the micro-DST of the BaBar Experiment with ROOT",
    "url": "https://arxiv.org/abs/physics/0206067"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "4dc7fc28-2ab9-48f5-981a-1295be027238",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}