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Gamma-ray burst detection capabilities of comptel

Authors :
James M. Ryan
W. Webber
V. Schönfelder
B. N. Swanenburg
Roland Diehl
A.V. Dordrecht
K. Bennett
B. G. Taylor
A. Aarts
G. Simpson
G. G. Lichti
C. Winkler
J. A. Lockwood
W. Hermsen
A. Deerenberg
Helmut Steinle
Source :
Advances in Space Research. 6:113-117
Publication Year :
1986
Publisher :
Elsevier BV, 1986.

Abstract

The imaging gamma-ray telescope COMPTEL, capable of detecting gamma rays in the 1 to 30 MeV range, is one of four experiments onboard NASA's Gamma-Ray Observatory GRO. Besides its primary objectives COMPTEL will contribute to the understanding of cosmic gamma-ray bursts. Summarising, COMPTEL localises bursts (S (E > 1 MeV) ≥ 2.10 −6 erg/cm 2 ) within 1 sr FOV to better than 1° at medium gamma-ray energies, measures continuum energy spectra in the range 0.1 MeV to 20 MeV with fluence S ≥ 6.9 10 −7 erg/cm 2 (5 σ , E≥100 keV), measures gamma-ray lines with detector resolution 9.6% (at 0.5 MeV) and 7.0% (at 1.5 MeV) and determines time histories of both gamma-ray line and continuum emission with t ≥ 0.1 sec resolution.

Details

ISSN :
02731177
Volume :
6
Database :
OpenAIRE
Journal :
Advances in Space Research
Accession number :
edsair.doi...........adc2a8495e9a0ad729204e63340987e6
Full Text :
https://doi.org/10.1016/0273-1177(86)90249-8