Hard X-ray optics for the HEFT balloon borne payload: Prototype design & status
被引:30
作者:
Craig, WW
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Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USAColumbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
Craig, WW
[1
]
Christensen, FE
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Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USAColumbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
Christensen, FE
[1
]
Decker, T
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Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USAColumbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
Decker, T
[1
]
Hailey, CJ
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Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USAColumbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
Hailey, CJ
[1
]
Harrison, FA
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Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USAColumbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
Harrison, FA
[1
]
Hill, RM
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Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USAColumbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
Hill, RM
[1
]
Jimenez-Garate, M
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Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USAColumbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
Jimenez-Garate, M
[1
]
Mao, P
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Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USAColumbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
Mao, P
[1
]
Schindler, S
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Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USAColumbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
Schindler, S
[1
]
机构:
[1] Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
来源:
EUV, X-RAY, AND GAMMA-RAY INSTRUMENTATION FOR ASTRONOMY IX
|
1998年
/
3445卷
关键词:
D O I:
10.1117/12.330269
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We report on the current status and performance of prototype hard X-ray optics we are producing for use on the High Energy Focusing Telescope (HEFT) experiment. The baseline substrates are thermally fanned glass mirrors that are overcoated with multilayers to provide good performance throughout the 20-80 keV bandpass. Progress made in the thermal forming process as well as in the multilayer performance has allowed production of optics that meet or exceed all HEFT requirements. We present metrology on the substrates and results from X-ray characterization. A novel mounting scheme for the individual telescope shells is currently being tested. If successful the mounting technique will produce a monolithic, extremely stiff and robust optic.