{
  "annotation_id": "f01af6ae-8217-431a-ac95-0007845e9ccb",
  "date_created": "2026-02-17T05:53:04.061000Z",
  "date_modified": "2026-02-17T05:53:04.061000Z",
  "file_hash": "2b407316b985016927c3029281d4048e4ecff60b0bbfbb382db63da7d2d60bf9",
  "private": false,
  "record": {
    "abstract": "We propose to radically expand the use of extragalactic globular clusters as tools for extragalactic archaeology. We propose a large-scale spectroscopic facility to obtain high spectral resolution (R $\\sim$ 20,000) spectroscopy for a significant fraction of all globular clusters in the nearby Universe. This will facilitate the reconstruction of galaxy assembly histories via chemical tagging, trace dark matter haloes, and measure extragalactic distances.",
    "arxiv_id": "2601.05849",
    "authors": [
      "M. A. Beasley",
      "K. Fahrion",
      "A. Gvozdenko",
      "S. Larsen"
    ],
    "categories": [
      "astro-ph.GA"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "title": "Extragalactic archaeology through high-resolution integrated-light spectroscopy of globular clusters",
    "url": "https://arxiv.org/abs/2601.05849",
    "version": "v1"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "3b12f016-7802-4179-8e8d-b3f2c7f86ce8",
    "id": "arXiv Dataset",
    "type": "Model",
    "variant": "snapshot-2026-01-17",
    "version": "0.1.0"
  },
  "user_id": 1000002
}