Simulations of GRB imaging with AGILE

Details Simulations of GRB imaging with AGILE Simulations of GRB imaging with AGILE

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..312..532l&link_type=abstract

Third Rome Workshop on Gamma-Ray Bursts in the Afterglow Era ASP Conference Series, Volume 312, Proceedings of the conference he

Astronomy and Astrophysics

Astrophysics

Scientific paper

AGILE is planned to be operational during the years 2005-2007. No other missions dedicated to gamma-ray astrophysics in the energy band 30 MeV - 50 GeV will be operational in that period. Most useful to GRB science will be the excellent positioning and sensitivity at off-axis angles, the very small instrumental deadtimes and the onboard capability to trigger GRB in the hard-X ray range. AGILE will be able to detect 5-10 events/year above 50 MeV and 1-2/month in the 10-40 keV energy range. AGILE will have the unique capability to study simultaneously the gamma-ray and the hard-X ray emission. Simulation results of the AGILE GRB imaging capability are presented.

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