{
  "@type": "dcat:Dataset",
  "accessLevel": "public",
  "accrualPeriodicity": "irregular",
  "bureauCode": [
    "026:00"
  ],
  "contactPoint": {
    "@type": "vcard:Contact",
    "fn": "Phil Newman",
    "hasEmail": "mailto:panewman@lheapop.gsfc.nasa.gov"
  },
  "description": "Since it is not possible to predict when a Gamma-Ray Burst (GRB) occurs, the follow-up ground telescopes must be distributed as uniform as possible all over the world in order to collect simultaneous data with the Swift detections. Based on the three-year operations of Swift, however, we noticed the distinct gap in follow-up coverage in the eastern U.S. region (Figure 1). This fact motivated us to construct a fully automated optical telescope here at GSFC.",
  "distribution": [
    {
      "@type": "dcat:Distribution",
      "downloadURL": "http://asd.gsfc.nasa.gov/Takanori.Sakamoto/GRT/",
      "format": "HTML",
      "mediaType": "text/html"
    }
  ],
  "identifier": "NASA-0000239",
  "issued": "2018-06-25",
  "keyword": [
    "active-galactic-nuclei",
    "gamma-ray-bursts",
    "grt",
    "jet-physics",
    "robotics",
    "telescope"
  ],
  "landingPage": "https://data.nasa.gov/dataset/goddard-robotic-telescope-grt",
  "modified": "2025-04-23",
  "programCode": [
    "026:014"
  ],
  "publisher": {
    "@type": "org:Organization",
    "name": "National Aeronautics and Space Administration"
  },
  "theme": [
    "Space Science"
  ],
  "title": "Goddard Robotic Telescope (GRT)"
}