Calibration of the first XMM flight mirror module - II - Effective area

被引：14

作者：

Gondoin, P ^{[1
]}

Aschenbach, B ^{[1
]}

Beijersbergen, M ^{[1
]}

Egger, R ^{[1
]}

Jansen, F ^{[1
]}

Stockman, Y ^{[1
]}

Tock, JP ^{[1
]}

机构：

[1] European Space Agcy, European Space Res & Technol Ctr, NL-2200 AG Noordwijk, Netherlands

来源：

X-RAY OPTICS, INSTRUMENTS, AND MISSIONS | 1998年 / 3444卷

关键词：

XMM; X-ray astronomy; Wolter I telescope; grazing incidence optics;

D O I：

10.1117/12.331244

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The High Throughput X-ray Spectroscopy Mission (XMM) is a "Cornerstone" Project in the ESA long-term Programme for Space Science. The satellite observatory uses three grazing incidence mirror modules coupled to reflection grating spectrometers and X-ray CCD cameras. Each XMM mirror module consists of 58 Welter I mirrors which are nested in a coaxial and cofocal configuration. The calibration of the mirror system includes the development of a representative numerical model and its validation against extensive calibration tests performed on ground at the CSL and PANTER test facilities. The present paper describes the calibration of the x-ray effective area of the first XMM flight mirror module.

引用

页码：290 / 301

页数：12

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