The University of Durham Mark 6 gamma ray telescope

被引：32

作者：

Armstrong, P ^{[1
]}

Chadwick, PM ^{[1
]}

Cottle, PJ ^{[1
]}

Dickinson, JE ^{[1
]}

Dickinson, MR ^{[1
]}

Dipper, NA ^{[1
]}

Hilton, SE ^{[1
]}

Hogg, W ^{[1
]}

Holder, J ^{[1
]}

Kendall, TR ^{[1
]}

McComb, TJL ^{[1
]}

Moore, CM ^{[1
]}

Orford, KJ ^{[1
]}

Rayner, SM ^{[1
]}

Roberts, ID ^{[1
]}

Roberts, MD ^{[1
]}

Robertshaw, M ^{[1
]}

Shaw, SE ^{[1
]}

Tindale, K ^{[1
]}

Tummey, SP ^{[1
]}

Turver, KE ^{[1
]}

机构：

[1] Univ Durham, Sci Labs, Dept Phys, Durham DH1 3LE, England

来源：

EXPERIMENTAL ASTRONOMY | 1999年 / 9卷 / 02期

关键词：

atmospheric Cerenkov technique; gamma ray astronomy; gamma ray telescopes;

D O I：

10.1023/A:1008018503904

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The design, construction and operation of the University of Durham ground-based gamma ray telescope is discussed. The telescope has been designed to detect gamma rays in the less than or equal to 200 GeV region and to achieve good discrimination between gamma ray and hadron initiated showers in the higher energy region (greater than or similar to 300 GeV). The telescope was commissioned in 1995 and a description of its design and operation is presented, together with a verification of the telescope's performance.

引用

页码：51 / 80

页数：30

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