{
  "id": "1610.06460",
  "version": "v1",
  "published": "2016-10-20T15:35:57.000Z",
  "updated": "2016-10-20T15:35:57.000Z",
  "title": "On the detectability of solar-like oscillations with the NASA TESS mission",
  "authors": [
    "Tiago L. Campante"
  ],
  "comment": "Submitted to EPJ Web of Conferences, to appear in the Proceedings of the joint TASC2/KASC9 workshop - SPACEINN & HELAS8 conference; 5 pages, 4 figures",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "The upcoming NASA TESS mission will perform an all-sky survey for planets transiting bright nearby stars. In addition, its excellent photometric precision will enable asteroseismology of solar-type and red-giant stars. We apply a newly developed detection test along a sequence of stellar evolutionary tracks in order to predict the detectability of solar-like oscillations with TESS.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2016-10-20T15:35:57.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "solar-like oscillations",
      "detectability",
      "planets transiting bright nearby stars",
      "stellar evolutionary tracks",
      "excellent photometric precision"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 5,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}