{"@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)"}