Production and calibration of the first HEFT hard X-ray optics module

被引:17
作者
Koglin, JE [1 ]
Chen, CMH [1 ]
Chonko, J [1 ]
Christensen, FE [1 ]
Craig, WW [1 ]
Decker, TR [1 ]
Gunderson, KS [1 ]
Hailey, CJ [1 ]
Harrison, FA [1 ]
Jensen, CP [1 ]
Madsen, KK [1 ]
Stern, M [1 ]
Windt, DL [1 ]
Yu, HT [1 ]
Ziegler, E [1 ]
机构
[1] Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
来源
OPTICS FOR EUV, X-RAY AND GAMMA-RAY ASTRONOMY | 2004年 / 5168卷
关键词
hard X-ray telescope; X-ray optics; segmented glass; thermally-slumped;
D O I
10.1117/12.506431
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Complete hard X-ray optics modules are currently being produced for the High Energy Focusing Telescope (HEFT), a balloon born mission that will observe a wide range of objects including young supernova remnants, active galactic nuclei, and galaxy clusters at energies between 20 and 70 keV. Large collecting areas are achieved by tightly nesting layers of grazing incidence mirrors in a conic approximation Wolter-I design. The segmented layers are made of thermally-formed glass substrates coated with depth-graded multilayer films for enhanced reflectivity. Our novel mounting technique involves constraining these mirror segments to successive layers of precisely machined graphite spacers. We report the production and calibration of the first HEFT optics module.
引用
收藏
页码:100 / 111
页数:12
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