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The Fermi Gamma-Ray Space Telescope: Overview and early science results
2009 IEEE Aerospace conference, 2009The Fermi Gamma-ray Space Telescope (formerly named GLAST) was designed and built by NASA, the United States Department of Energy, and agencies in France, Germany, Italy, Japan and Sweden. It launched in June of 2008 and has been observing the gamma-ray sky for over 6 months.
Mark Seidleck +2 more
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Fermi Gamma-ray Space Telescope: Highlights of the GeV Sky
Nuclear Physics B - Proceedings Supplements, 2011Because high-energy gamma rays can be produced by processes that also produce neutrinos. the gamma-ray survey of the sky by the Fermi Gamma-ray Space Telescope offers a view of potenl ial targds for neutrino observations. Gamma-ray bursts. active galactic nuclei, and supernova remnants are all sites where hadronic, neutrino-producing interactions are ...
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Viewing the High-Energy Universe with the Fermi Gamma-ray Space Telescope
Frontiers in Optics 2010/Laser Science XXVI, 2010The Fermi Gamma-ray Space Telescope has completed 2 years of observations of the entire sky from 10 keV to more than 300 GeV, providing a new view of the high-energy Universe.
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First light from the Vela pulsar with the Fermi Gamma-ray Space Telescope
AIP Conference Proceedings, 2009The Fermi Gamma‐ray Space Telescope, launched in June 2008, is an international space mission entirely devoted to the study of the high‐energy gamma rays from the Universe. The main instrument aboard Fermi is the Large Area Telescope (LAT), a pair conversion telescope equipped with the state‐of‐the art in gamma‐ray detectors technology.
M. Razzano +2 more
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Status of the technology of the current space missions including the Fermi gamma-ray space telescope
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2010Abstract We review the status of X-rays and γ -rays space missions operational in 2009. We provide highlights of the current semiconductor technology instrumentation and briefly discuss challenges to be addressed by future missions.
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Fermi Gamma-ray Space Telescope, Introduction and Highlights from the First Eight Months
AIP Conference Proceedings, 2009The Fermi Gamma‐ray Space Telescope, formerly named GLAST, is a mission in low‐Earth orbit to observe gamma rays from the cosmos in the broad energy range from 20 MeV to >300 GeV, with supporting observations of gamma‐ray bursts from 8 keV to 30 MeV. The telescope far surpasses previous generations in its ability to detect and localize faint gamma‐ray ...
R. P. Johnson, Marvin L. Marshak
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Some highlights of the first four years of the Fermi Gamma-ray Space Telescope
Frontiers of Physics, 2013The Fermi Gamma-ray Space Telescope, formerly called GLAST, measures the cosmic gamma-ray flux in the energy range 8 keV to > 300 GeV. In addition to breakthrough capabilities in energy coverage and localization, the very large field of view enables observations of 20% of the sky at any instant, and the entire sky on a timescale of a few hours.
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THE FERMI GAMMA-RAY SPACE TELESCOPE: PERFORMANCE AND RESULTS AT THE 1-YEAR MILESTONE
Astroparticle, Particle and Space Physics, Detectors and Medical Physics Applications, 2010openaire +2 more sources