EXIST'S gamma-ray burst sensitivity

  • D. L. Band
  • , J. E. Grindlay
  • , J. Hong
  • , G. Fishman
  • , D. H. Hartmann
  • , A. Garson
  • , H. Krawczynski
  • , S. Barthelmy
  • , N. Gehrels
  • , G. Skinner

Research output: Contribution to journalArticlepeer-review

10 Scopus citations

Abstract

We use semianalytic techniques to evaluate the burst sensitivity of designs for the EXIST hard X-ray survey mission. Applying these techniques to the mission design proposed for the Beyond Einstein program, we find that with its very large field of view and faint gamma-ray burst detection threshold, EXIST will detect and localize approximately two bursts per day, a large fraction of which may be at high redshift. We estimate that EXIST's maximum sensitivity will be ∼4 times greater than that of Swift's Burst Alert Telescope. Bursts will be localized to better than 40″ at threshold, with a burst position as good as a few arcseconds for strong bursts. EXIST's combination of three different detector systems will provide spectra from 3 keV to more than 10 MeV. Thus, EXIST will enable a major leap in the understanding of bursts, their evolution, environment, and utility as cosmological probes.

Original languageEnglish
Pages (from-to)1225-1232
Number of pages8
JournalAstrophysical Journal
Volume673
Issue number2
DOIs
StatePublished - Feb 1 2008

Keywords

  • Gamma rays: bursts

Fingerprint

Dive into the research topics of 'EXIST'S gamma-ray burst sensitivity'. Together they form a unique fingerprint.

Cite this