Published September 28, 2004 | Version Published
Book Section - Chapter Open

Observing GRBs with EXIST

  • 1. ROR icon Clemson University
  • 2. ROR icon Harvard-Smithsonian Center for Astrophysics
  • 3. ROR icon Stanford University
  • 4. ROR icon Lawrence Livermore National Laboratory
  • 5. ROR icon National Aeronautics and Space Administration
  • 6. ROR icon National Space Science and Technology Center
  • 7. ROR icon Goddard Space Flight Center
  • 8. ROR icon California Institute of Technology
  • 9. ROR icon University of California, Santa Cruz

Contributors

Abstract

We describe the Energetic X-ray Imaging Survey Telescope EXIST, designed to carry out a sensitive all-sky survey in the 10 keV – 600 keV band. The primary goal of EXIST is to find black holes in the local and distant universe. EXIST also traces cosmic star formation via gamma-ray bursts and gamma-ray lines from radioactive elements ejected by supernovae and novae.

Additional Information

© 2004 American Institute of Physics. Issue Date: 28 September 2004.

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Identifiers

Eprint ID
12271
Resolver ID
CaltechAUTHORS:HARaipcp04

Dates

Created
2008-10-31
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Updated
2021-11-08
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Caltech Custom Metadata

Caltech groups
Space Radiation Laboratory
Series Name
American Institute of Physics Conference Proceedings
Series Volume or Issue Number
727