{
  "id": "2001.03497",
  "version": "v1",
  "published": "2020-01-10T15:09:39.000Z",
  "updated": "2020-01-10T15:09:39.000Z",
  "title": "The prototype star $γ$ Doradus observed by TESS",
  "authors": [
    "S. Christophe",
    "V. Antoci",
    "E. Brunsden",
    "R. -M. Ouazzani",
    "S. J. A. J. Salmon"
  ],
  "comment": "2 pages, 2 figures, poster contribution at the conference \"Stars and their variability observed from space - Celebrating the 5th anniversary of BRITE-Constellation\", Vienna, Austria, August 19 - 23, 2019. Eds: C. Neiner, W. Weiss, D. Baade, E. Griffin, C. Lovekin, A. Moffat",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "$\\gamma$ Doradus is the prototype star for the eponymous class of pulsating stars that consists of late A-early F main-sequence stars oscillating in low-frequency gravito-inertial modes. Being among the brightest stars of its kind (V = 4.2), $\\gamma$ Dor benefits from a large set of observational data that has been recently completed by high-quality space photometry from the TESS mission. With these new data, we propose to study $\\gamma$ Dor as an example of possibilities offered by synergies between multi-technical ground and space-based observations. Here, we present the preliminary results of our investigations.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2020-01-10T15:09:39.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "prototype star",
      "low-frequency gravito-inertial modes",
      "high-quality space photometry",
      "brightest stars",
      "main-sequence stars"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 2,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}