The IBIS gamma-ray telescope on INTEGRAL

被引：0

作者：

Ubertini, P ^{[1
]}

Lebrun, F ^{[1
]}

Di Cocco, G ^{[1
]}

Bassani, L ^{[1
]}

Bazzano, A ^{[1
]}

Bird, AJ ^{[1
]}

Broenstad, K ^{[1
]}

Caroli, E ^{[1
]}

Cocchi, M ^{[1
]}

De Cesare, G ^{[1
]}

Denis, M ^{[1
]}

Di Cosimo, S ^{[1
]}

Di Lellis, A ^{[1
]}

Giannotti, F ^{[1
]}

Goldoni, P ^{[1
]}

Goldwurm, A ^{[1
]}

La Rosa, G ^{[1
]}

Labanti, C ^{[1
]}

Laurent, P ^{[1
]}

Limousin, O ^{[1
]}

Malaguti, G ^{[1
]}

Mirabel, IF ^{[1
]}

Natalucci, L ^{[1
]}

Orleansky, P ^{[1
]}

Poulsen, MJ ^{[1
]}

Quadrini, M ^{[1
]}

Ramsey, B ^{[1
]}

Reglero, V ^{[1
]}

Sabau, L ^{[1
]}

Sacco, B ^{[1
]}

Santangelo, A ^{[1
]}

Segreto, A ^{[1
]}

Staubert, R ^{[1
]}

Stephen, J ^{[1
]}

Trifoglio, M ^{[1
]}

Vigroux, L ^{[1
]}

Volkmer, R ^{[1
]}

Weisskopf, MC ^{[1
]}

Zdziarski, A ^{[1
]}

Zehnder, A ^{[1
]}

机构：

[1] CNR, IAS, Rome, Italy

来源：

FIFTH COMPTON SYMPOSIUM | 2000年 / 510卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 (similar to 3,000 cm(2)) multilayer detector which utilises both Cadmium Telluride (16,384 detectors) and Caesium Iodide elements (4,096 detectors) to provide the fine angular resolution similar to 12 arcmin, wide spectral response (20 keV to 10 MeV), high resolution timing (61 mu s) 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].

引用

页码：684 / 688

页数：5

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