{
  "annotation_id": "d387c205-b832-4d68-89a1-1a102a29d021",
  "date_created": "2026-03-02T18:00:53.423000Z",
  "date_modified": "2026-03-02T18:00:53.423000Z",
  "file_hash": "954ce6aa8d06950f92d7d5db474fa0d3e06faabb2e4c9319ea8d1535e3cf09dc",
  "private": false,
  "record": {
    "abstract": "IR spectra gained from laboratory investigations on analogue materials are an\nimportant tool for the interpretation of astronomical IR data and the\nunderstanding of the observed phenomena in DISM. Dust particles grown in\nargon/acetylene low pressure plasma are proposed for a new analog. We test the\nvalidity of proposed analog according to the criteria from the literature. We\nalso present preliminary results of nitrogen band at 4.62 \\$mu$m, which has\nbeen identified in dense cold dust.",
    "arxiv_id": "physics/0410083",
    "authors": [
      "Ilija Stefanovic",
      "Eva Kovacevic",
      "Johannes Berndt",
      "Yvonne Pendleton",
      "Jorg Winter"
    ],
    "categories": [
      "physics.plasm-ph"
    ],
    "title": "Nanoparticles designed from low pressure plasma as model for   astrophysical dust clouds",
    "url": "https://arxiv.org/abs/physics/0410083"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "49d76c29-52dc-4f7b-a829-237e5b2cd1b3",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}