{
  "id": "1806.07270",
  "version": "v1",
  "published": "2018-06-18T17:22:12.000Z",
  "updated": "2018-06-18T17:22:12.000Z",
  "title": "Revealing the Galactic Population of BHs",
  "authors": [
    "Thomas J. Maccarone",
    "Laura Chomiuk",
    "Jay Strader",
    "James Miller-Jones",
    "Greg Sivakoff"
  ],
  "comment": "9 pages, article for ngVLA Science Book",
  "categories": [
    "astro-ph.HE",
    "astro-ph.SR"
  ],
  "abstract": "We discuss the case for using the Next Generation Very Large Array both to discover new black hole X-ray binaries astrometrically, and to characterize them. We anticipate that the ngVLA will be able to find $\\sim$100 new black hole X-ray binaries, as well as a host of other interesting radio stars, in a few hundred hour survey. Parallax and astrometric wobble measurements will be achievable in feasible follow-up surveys especially using long baseline capabilities. The ngVLA's high angular resolution, high survey speed, and high frequency sensitivity give it a unique range of parameter space over which it is sensitive.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2018-06-18T17:22:12.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "black hole x-ray binaries",
      "galactic population",
      "ngvlas high angular resolution",
      "high frequency sensitivity",
      "long baseline capabilities"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 9,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}