The Gamma-ray Large Area Space Telescope (GLAST) Mission

Details The Gamma-ray Large Area Space Telescope (GLAST) Mission The Gamma-ray Large Area Space Telescope (GLAST) Mission

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.9801r&link_type=abstract

American Astronomical Society, AAS Meeting #211, #98.01; Bulletin of the American Astronomical Society, Vol. 39, p.909

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The Gamma-ray Large Area Space Telescope, GLAST, is a mission to measure the cosmic gamma-ray flux in the energy range 20 MeV to >300; GeV, with supporting measurements for gamma-ray bursts from 8 keV to 30 MeV. The very large field of view will make it possible to observe 20% of the sky at any instant, and the entire sky on a timescale of a few hours. With its launch in 2008, GLAST will open a new and important window on a wide variety of phenomena, including black holes and active galactic nuclei; the optical-UV extragalactic background light, gamma-ray bursts; the origin of cosmic rays and supernova remnants; and searches for hypothetical new phenomena such as supersymmetric dark matter annihilations and Lorentz invariance violation. In addition to the science opportunities, this poster includes a description of the instruments, the opportunities for guest observers, and the mission status.

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