The INTEGRAL mass model - TIMM

被引:21
作者
Ferguson, C [1 ]
Barlow, EJ
Bird, AJ
Dean, AJ
Hill, AB
Shaw, SE
Stephen, JB
Sturner, S
Tikkanen, TV
Weidenspointner, G
Willis, DR
机构
[1] Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England
[2] CNR, IASF, I-40129 Bologna, Italy
[3] NASA, Goddard Space Flight Ctr, LHEA, Greenbelt, MD 20771 USA
[4] Univ Space Res Assoc, Lanham, MD 20706 USA
[5] Ctr Etud Spatiale Rayonnements, F-31028 Toulouse 4, France
来源
ASTRONOMY & ASTROPHYSICS | 2003年 / 411卷 / 01期
关键词
gamma-ray astronomy; instrument simulation;
D O I
10.1051/0004-6361:20031403
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The INTEGRAL Mass Model (TIMM) was started in 1995 and aimed to create a detailed geometrical model of the whole INTEGRAL satellite on computer. In parallel, a comprehensive Monte Carlo simulation code (called GGOD) has been developed. The mass model and the Monte Carlo code together enable the in-flight operation of INTEGRAL to be simulated at the individual event level. Thus TIMM can be used to provide an independent evaluation of the performance of the individual instruments, to study the interference and complementarity between instruments, to generate test data for software development, and as a powerful tool for post-launch diagnosis. In this paper TIMM is briefly reviewed, some examples from ground calibration are presented, and preliminary comparison to flight data is shown. The future use of TIMM to flat field flight data is also briefly discussed.
引用
收藏
页码:L19 / L23
页数:5
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