{
  "annotation_id": "c4da3dc6-b3b4-4e23-b68c-2ee6f8e24f46",
  "date_created": "2026-03-02T18:00:56.754000Z",
  "date_modified": "2026-03-02T18:00:56.754000Z",
  "file_hash": "d2eb14aa2b227467ecf24808987df3feb7117b76f3ce3c38e6ca71c1ddb46026",
  "private": false,
  "record": {
    "abstract": "At the beginning of a class or meeting an icebreaker activity is often used\nto help loosen the group and get everyone talking. Our motivation is to develop\nactivities that serve the purpose of an icebreaker, but are designed to enhance\nand supplement a science-oriented agenda. The subject of this article is an\nicebreaker activity related to gravitational wave astronomy. We first describe\nthe unique gravitational wave signals from three distinct sources:\nmonochromatic binaries, merging compact objects, and extreme mass ratio\nencounters. These signals form the basis of the activity where participants\nwork to match an ideal gravitational wave signal with noisy detector output for\neach type of source.",
    "arxiv_id": "physics/0503198",
    "authors": [
      "Michelle B. Larson",
      "Louis J. Rubbo",
      "Kristina D. Zaleski",
      "Shane L. Larson"
    ],
    "categories": [
      "physics.ed-ph"
    ],
    "doi": "10.1119/1.2353577",
    "title": "Science Icebreaker Activities: An Example from Gravitational Wave   Astronomy",
    "url": "https://arxiv.org/abs/physics/0503198"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "70c14eb2-c9fe-4835-a869-e51a914987da",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}