{
  "annotation_id": "b20ec5e9-2899-4b00-91f4-134c7a0a9d3a",
  "date_created": "2026-03-02T18:01:00.600000Z",
  "date_modified": "2026-03-02T18:01:00.600000Z",
  "file_hash": "d02470b7e4f6724dc046dda9e3ac5e99b068d13061270d596ca2380fd263f630",
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  "record": {
    "abstract": "This article reviews the current status of gravitational wave astronomy and\nexplains why astronomers are excited about the new generation of gravitational\nwave detectors. As part of the review we compare and contrast gravitational\nradiation to the more familiar electromagnetic radiation. We discuss the\ncurrent indirect experimental evidence for gravitational waves, and how current\nand future gravitational wave detectors will operate as our newest telescopes\npointed at the skies.",
    "arxiv_id": "physics/0509201",
    "authors": [
      "Louis J. Rubbo",
      "Shane L. Larson",
      "Michelle B. Larson",
      "Kristina D. Zaleski"
    ],
    "categories": [
      "physics.ed-ph"
    ],
    "doi": "10.1119/1.2353578",
    "title": "Gravitational Waves: new observatories for new astronomy",
    "url": "https://arxiv.org/abs/physics/0509201"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "8d8767d8-673b-499c-b384-690563ee8bc6",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}