{
  "id": "2502.06198",
  "version": "v1",
  "published": "2025-02-07T14:15:37.000Z",
  "updated": "2025-02-07T14:15:37.000Z",
  "title": "Ultracool dwarfs in Gaia",
  "authors": [
    "Céline Reylé"
  ],
  "comment": "Evry Schatzman School 2023: Stellar physics with Gaia",
  "journal": "EES2023: Proceedings of the Evry Schatzman School. Eds.: Babusiaux, C.; Reyl\\'e, C",
  "categories": [
    "astro-ph.SR",
    "astro-ph.GA"
  ],
  "abstract": "The Gaia optical observations are not the most suitable spectral domain for studying the low-mass, faintest and reddest part of the main sequence. Nevertheless, the large number of objects observed with an unprecedented precision, including trigonometric parallax, makes it an unrivaled dataset for studying the stellar-substellar boundary. In this paper, I review the contribution of the successive catalogues offered by the Gaia mission to study the low-mass, ultra-cool objetcs. I also present further characterisations and scientific exploitations of the Gaia sample.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2025-02-07T14:15:37.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "ultracool dwarfs",
      "reddest part",
      "main sequence",
      "gaia sample",
      "gaia optical observations"
    ],
    "tags": [
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}