Estimation of GRB detection by FiberGLAST

Details Estimation of GRB detection by FiberGLAST Estimation of GRB detection by FiberGLAST

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..526..706p&link_type=abstract

GAMMA-RAY BURSTS: 5th Huntsville Symposium. AIP Conference Proceedings, Volume 526, pp. 706-710 (2000).

Physics

Spectroscopy And Spectrophotometry, X-Ray, Jets And Bursts, Galactic Winds And Fountains

Scientific paper

FiberGLAST is one of several instrument concepts being developed for possible inclusion as the primary Gamma-ray Large Area Space Telescope (GLAST) instrument. The predicted FiberGLAST effective area is more than 12,000 cm2 for energies between 30 MeV and 300 GeV, with a field of view that is essentially flat from 0°-80°. The detector will achieve a sensitivity more than 10 times that of EGRET. We present results of simulations that illustrate the sensitivity of FiberGLAST for the detection of gamma-ray bursts. .

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