Published September 28, 2004 | Version v1
Journal article

Observing GRBs with EXIST

  • 1. Department of Physics and Astronomy, Clemson University, Clemson, SC (United States)
  • 2. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  • 3. Stanford Linear Accelerator, Stanford University, Stanford, CA (United States)
  • 4. Lawrence Livermore National Laboratory, Livermore, CA (United States)
  • 5. NSSTC, Huntsville, AL (United States)
  • 6. NASA, Marshal Space Flight Center, Huntsville, AL (United States)
  • 7. NASA, Goddard Space Flight Center, Greenbelt, MD (United States)
  • 8. California Institute of Technology, Pasadena, CA (United States)
  • 9. Dept. of Astronomy and Astrophysics, University of California, Santa Cruz, CA (United States)

Description

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 details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
727
Journal Issue
1
Journal Page Range
p. 677-680
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
30 years of discovery
Acronym
Symposium on gamma-ray bursts
Dates
8-12 Sep 2003
Place
Santa Fe, NM (United States)

Optional Information

Notes
(c) 2004 American Institute of Physics