MISO LOW-ENERGY GAMMA-RAY TELESCOPE

被引：21

作者：

BAKER, RE ^{[1
]}

BUTLER, RC ^{[1
]}

DEAN, AJ ^{[1
]}

DICOCCO, G ^{[1
]}

DIPPER, NA ^{[1
]}

MARTIN, SJ ^{[1
]}

MOUNT, KE ^{[1
]}

RAMSDEN, D ^{[1
]}

BARBAGLIA, G ^{[1
]}

BARBARESCHI, L ^{[1
]}

BOELLA, G ^{[1
]}

BUSSINI, A ^{[1
]}

IGIUNI, A ^{[1
]}

INZANI, P ^{[1
]}

PEROTTI, F ^{[1
]}

VILLA, G ^{[1
]}

机构：

[1] CNR,FIS COSM & TECNOL RELAT LAB,I-20133 MILAN,ITALY

来源：

NUCLEAR INSTRUMENTS & METHODS | 1979年 / 158卷 / 2-3期

关键词：

D O I：

10.1016/S0029-554X(79)96375-4

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

This paper describes the balloon-flight version of a low energy (0.2-20 MeV) gamma-ray telescope developed in collaboration by the Milan and Southampton groups. The instrument embodies a Compton-coincidence system comprising an upper liquid scintillator and a large sodium iodide crystal (560 cm2). This detector is mounted inside a semiactive shielding system which collimates the incident photons (1.5° fwhm). The telescope is mounted in an orientation system which has a pointing accuracy of better than 0.5°. The instrument has been extensively tested using beams of γ-rays, neutrons and high energy protons (2 GeV/c). © 1979 North-Holland Publishing Co.

引用

页码：595 / 604

页数：10

共 32 条

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