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The IBIS Gamma-Ray telescope on INTEGRAL.

Authors :
Ubertini, P.
Lebrun, F.
Di Cocco, G.
Bassani, L.
Bazzano, A.
Bird, A. J.
Broenstad, K.
Caroli, E.
Cocchi, M.
De Cesare, G.
Denis, M.
Di Cosimo, S.
Di Lellis, A.
Giannotti, F.
Goldoni, P.
Goldwurm, A.
La Rosa, G.
Labanti, C.
Laurent, P.
Limousin, O.
Source :
AIP Conference Proceedings; 2000, Vol. 510 Issue 1, p684, 5p, 1 Black and White Photograph, 2 Diagrams, 1 Graph
Publication Year :
2000

Abstract

The IBIS Telescope is the high angular resolution Gamma-Ray imager on-Board the INTEGRAL Satellite. IBIS features a coded aperture mask and a novel large area (∼3,000 cm2) multilayer detector which utilises both Cadmium Telluride (16,384 detectors) and Caesium Iodide elements (4,096 detectors) to provide the fine angular resolution ∼12 arcmin, wide spectral response (20 keV to 10 MeV), high resolution timing (61 μs) and spectroscopy (6% at 100 keV) required to satisfy the mission’s imaging objectives. This paper will focus on the IBIS hardware characteristics while the Scientific Performance of the telescope have been recently addressed elsewhere [1]. © 2000 American Institute of Physics. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
0094243X
Volume :
510
Issue :
1
Database :
Complementary Index
Journal :
AIP Conference Proceedings
Publication Type :
Conference
Accession number :
6029707