Published April 12, 2000 | Version v1
Journal article

EXIST: A high sensitivity hard x-ray imaging sky survey mission for ISS

  • 1. MIT (US)
  • 2. IOA/Cambridge (US)
  • 3. Rome Obs./BeppoSAX (IT)
  • 4. NASA/GSFC (US)
  • 5. Columbia Univ. (US)
  • 6. Caltech (US)
  • 7. Clemson Univ. (US)
  • 8. NASA/MSFC (US)
  • 9. UCSD (US)
  • 10. Birmingham Univ./United Kingdom (GB)
  • 11. UC Santa Cruz (US)

Description

A deep all-sky imaging hard x-ray survey and wide-field monitor is needed to extend soft (ROSAT) and medium (ABRIXAS2) x-ray surveys into the 10-100 keV band at comparable sensitivity (∼0.05 mCrab). This would enable discovery and study of (greater-or-similar sign)3000 obscured AGN, which probably dominate the hard x-ray background; detailed study of spectra and variability of accreting black holes and a census of BHs in the Galaxy; Gamma-ray bursts and associated massive star formation (PopIII) at very high redshift and Soft Gamma-ray Repeaters throughout the Local Group; and a full galactic survey for obscured supernova remnants. The Energetic X-ray Imaging Survey Telescope (EXIST) is a proposed array of 8x1 m2 coded aperture telescopes fixed on the International Space Station (ISS) with 160 degree sign x40 degree sign field of view which images the full sky each 90 min orbit. EXIST has been included in the most recent NASA Strategic Plan as a candidate mission for the next decade. An overview of the science goals and mission concept is presented

Additional details

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
510
Journal Issue
1
Journal Page Range
p. 784-788
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
5. Compton symposium on gamma-ray astronomy
Dates
15-17 Sep 1999
Place
Portsmouth, NH (United States)

Optional Information

Notes
(c) 2000 American Institute of Physics.