{
    "count": 1,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 10426,
            "url": "https://svs.gsfc.nasa.gov/10426/",
            "result_type": "Produced Video",
            "release_date": "2009-07-02T13:50:00-04:00",
            "title": "Vela Pulsar in Gamma Rays",
            "description": "This movie shows pulsed gamma rays from the Vela pulsar as constructed from photons detected by Fermi's Large Area Telescope. The Vela pulsar, which spins 11 times a second, is the brightest persistent source of gamma rays in the sky. The movie includes data from August 4 to Sept. 15, 2008. The bluer color in the latter part of the pulse indicates the presence of gamma rays with energies exceeding a billion electron volts (1 GeV). For comparison, visible light has energies between two and three electron volts. Red indicates gamma rays with energies less than 300 million electron volts (MeV); green, gamma rays between 300 MeV and 1 GeV; and blue shows gamma rays greater than 1 GeV. The movie frame is 30 degrees across. The background, which shows diffuse gamma-ray emission from the Milky Way, is about 15 times brighter here than it actually is. || ",
            "hits": 88
        }
    ]
}