The Constellation X-ray mission: Implementation concept and science overview

被引:20
作者
Tananbaum, H [1 ]
White, NE [1 ]
Bookbinder, JA [1 ]
Marshall, FE [1 ]
Cordova, FA [1 ]
机构
[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
来源
EUV, X-RAY, AND GAMMA-RAY INSTRUMENTATION FOR ASTRONOMY X | 1999年 / 3765卷
关键词
X-rays; spectroscopy; Constellation-X; abundances;
D O I
10.1117/12.366555
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Constellation-X mission is a large collecting area X-ray facility, emphasizing observations at high spectral resolution (E/Delta E similar to 300-3000) while covering a broad energy band(0.25-40 keV). By increasing the telescope aperture and utilizing efficient spectrometers the mission will achieve a factor of 100 increased sensitivity over current high resolution ii-ray spectroscopy missions. The use of focussing optics across the 10-40 keV band will provide a similar factor of 100 increased sensitivity in this band. Key technologies under development for the mission include lightweight high throughput ii-ray optics, multilayer coatings to enhance the hard ii-ray performance of ii-ray optics, micro-calorimeter spectrometer arrays with 2 eV resolution,low power and low weight CCD arrays, lightweight gratings and hard ii-ray detectors. When observations commence towards the end of the next decade, Constellation-X will address many pressing questions concerning the extremes of gravity and the evolution of the Universe.
引用
收藏
页码:62 / 72
页数:11
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