{
  "annotation_id": "e5bc9327-64ad-4601-b00e-72f91d787767",
  "date_created": "2026-03-02T18:00:42.790000Z",
  "date_modified": "2026-03-02T18:00:42.790000Z",
  "file_hash": "45818a5d93c0c3c4e0441fb2ada733cfcbd119a9d7664e09c9b9f0db35f5844d",
  "private": false,
  "record": {
    "abstract": "The Grid technologies are in ongoing development. Using current Grid toolkits\nlike the Globus toolkit gives one the possibility to build up virtual\norganizations. Although these tookits are in still under development and do not\nfeature all functionality, they can already now be used to set up an efficient\ncomputing environment for physics collaborations with only moderate work. We\ndiscuss in this paper the use of such a computing structure in two running\nexperiments - the AMANDA (AMANDA = Antarctic muon and neutrino detector array)\nneutrino telescope and the D0 experiment at Tevatron, Fermilab. One of the main\nfeatures of our approach is to avoid reprogramming of the existing software\nwhich is based on several programming languages (FORTRAN, C/C++, JAVA). This\nwas realized with software layers around the collaboration software taking care\nabout in- and output, user notification, tracking of running jobs, etc. A\nfurther important aspect is the resolution of library dependencies, which occur\nwhen a user runs self-compiled jobs on machines, where these libraries are not\ninstalled. These dependencies are also resolved with this layers.",
    "arxiv_id": "physics/0305081",
    "authors": [
      "T. Harenberg",
      "K. -H. Becker",
      "W. Rhode",
      "C. Schmitt"
    ],
    "categories": [
      "physics.comp-ph",
      "hep-ex"
    ],
    "title": "AMANDA - first running experiment to use GRID in production",
    "url": "https://arxiv.org/abs/physics/0305081"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "3d3b6f34-8d77-4816-9bb3-a2003fbab473",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}