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Front. Phys.    0, Vol. Issue () : 693-713    https://doi.org/10.1007/s11467-013-0401-1
REVIEW ARTICLE
Some highlights of the first four years of the Fermi Gamma-ray Space Telescope
Steven Ritz()
Department of Physics and the SCIPP, University of California Santa Cruz, Santa Cruz, CA 95064, USA
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Abstract

The 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. With its launch in 2008, Fermi opens a new and important window on a wide variety of phenomena, including pulsars, black holes and active galactic nuclei, gamma-ray bursts, supernova remnants and the origins of cosmic rays, and searches for hypothetical new phenomena such as particle dark matter annihilations. A brief overview and selected science highlights from the first four years are provided.
Keywords high-energy gamma-ray astrophysics      dark matter      fundamental physics tests      spacebased astrophysics      space-based particle astrophysics      gamma-ray bursts      blazars      pulsars     
Corresponding Author(s): Ritz Steven,Email:sritz@ucsc.edu   
Issue Date: 01 December 2013
 Cite this article:   
Steven Ritz. Some highlights of the first four years of the Fermi Gamma-ray Space Telescope[J]. Front. Phys. , 0, (): 693-713.
 URL:  
https://academic.hep.com.cn/fop/EN/10.1007/s11467-013-0401-1
https://academic.hep.com.cn/fop/EN/Y0/V/I/693
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