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Fermi Gamma-Ray Space Telescope

机译:Fermi Gamma-Ray Space Telescope

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摘要

The Fermi Gamma-ray Space Telescope, launched in June 2008, is an observatory designed to survey the high-energy gamma-ray sky. The primary instrument, the Large Area Telescope (LAT), provides observations from 20 MeV to greater than 300 GeV. A second instrument, the Gamma-ray Burst Monitor (GBM), provides observations of transients from less than 10 keV to 40 MeV. We describe the design and performance of the instruments and their subsystems, the spacecraft and the ground system.

著录项

  • 来源
    《Optical Engineering》 |2012年第1期|011012-1-011012-9|共9页
  • 作者单位

    NASA Goddard Space Flight Center, Greenbelt, Maryland 20771;

    Stanford University, W. W. Hansen Experimental Physics Laboratory, Stanford, California, 94305-4085;

    University of Alabama in Huntsville, Huntsville, Center for Space Plasma and Aeronomic Research (CSPAR), Huntsville, Alabama 35899University of California, Santa Cruz Institute for Particle Physics, Santa Cruz, California 95064;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);
  • 原文格式 PDF
  • 正文语种 英语
  • 中图分类 计量学;
  • 关键词

    astronomy; gamma rays; silicon;

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