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Capability of the ASTRO-E Hard X-ray Detector for high-energy transients and γ-ray Bursts.

Authors :
Terada, Y.
Yamaoka, K.
Kokubun, M.
Kotoku, J.
Mizuno, T.
Kataoka, J.
Takahasi, T.
Murakami, T.
Makishima, K.
Kamae, T.
Source :
AIP Conference Proceedings. 2000, Vol. 510 Issue 1, p667. 4p. 1 Diagram, 2 Charts, 3 Graphs.
Publication Year :
2000

Abstract

The Hard X-Ray Detector (HXD) is one of the instruments on board ASTRO-E, scheduled for lanch in January–February 2000. The HXD consists of 16 Well-type phoswich counters, surrounded by 20 active shield counters (Anti Coincidence Counters: Anti–Counters). It covers the energy range 10–600 keV with a very low background. Because the Anti–Counters are made of thich high-Z material with a very large geometrical area, they retain a large effective area up to high energies. Therefore the Anti–Counters can be used for monitoring high-energy transient sources and γ-ray bursts. In this paper, the all sky monitoring function with the Anti–Counters and the result of their ground calibration tests are described. © 2000 American Institute of Physics. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
0094243X
Volume :
510
Issue :
1
Database :
Academic Search Index
Journal :
AIP Conference Proceedings
Publication Type :
Conference
Accession number :
6029710