Optimization of graded multilayer designs for astronomical X-ray telescopes
We developed a systematic method for optimizing the design of depth-graded multilayers for astronomical hard-x-ray and soft-gamma-ray telescopes based on the instrument's bandpass and the field of view. We apply these methods to the design of the conical-approximation Wolter I optics employed b...
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Published in | Applied optics (2004) Vol. 38; no. 22; p. 4766 |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
United States
01.08.1999
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Online Access | Get more information |
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Summary: | We developed a systematic method for optimizing the design of depth-graded multilayers for astronomical hard-x-ray and soft-gamma-ray telescopes based on the instrument's bandpass and the field of view. We apply these methods to the design of the conical-approximation Wolter I optics employed by the balloon-borne High Energy Focusing Telescope, using W/Si as the multilayer materials. In addition, we present optimized performance calculations of mirrors, using other material pairs that are capable of extending performance to photon energies above the W K-absorption edge (69.5 keV), including Pt/C, Ni/C, Cu/Si, and Mo/Si. |
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ISSN: | 1559-128X 2155-3165 |
DOI: | 10.1364/AO.38.004766 |