Development of the HEFT and NuSTAR focusing telescopes

被引:61
作者
Harrison, Fiona A. [1 ]
Christensen, Finn E.
Craig, William
Hailey, Charles
Baumgartner, Wayne
Chen, C. M. H.
Chonko, James
Cook, W. Rick
Koglin, Jason
Madsen, Kristin-Kruse
Pivavoroff, Michael
Boggs, Steven
Smith, David
机构
[1] CALTECH, Space Radiat Lab, Pasadena, CA 91125 USA
[2] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
[3] Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
[4] Univ Calif Berkeley, Berkeley, CA 94720 USA
[5] Univ Calif Santa Cruz, Santa Cruz, CA 95064 USA
关键词
X-ray telescopes; X-ray optics; X-ray detectors;
D O I
10.1007/s10686-006-9072-z
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Hard X-ray/soft gamma-ray astrophysics is on the verge of a major advance with the practical realization of technologies capable of efficiently focusing X-rays above 10 keV. Hard X-ray focusing telescopes can achieve orders of magnitude improvements in sensitivity compared to the instruments based on coded apertures and collimated detectors that have traditionally been employed in this energy band. Compact focal planes enable high-performance detectors with good spectral resolution to be employed in efficient, low-background configurations. We have developed multilayer coated grazing incidence optics and solid state Cadmium Zinc Telluride focal plane systems for the High Energy Focusing Telescope (HEFT) balloon-borne experiment, and for the Nuclear Spectroscopic Telescope Array (NuSTAR) Small Explorer satellite. In this paper we describe the technologies, telescope designs, and performance of both experiments.
引用
收藏
页码:131 / 137
页数:7
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