Craig, William W. and Hailey, Charles J. and Jimenez-Garate, Mario and Windt, David L. and Harrison, Fiona A. and Mao, Peter H. and Christensen, Finn E. and Hussain, Ahsen M. (2000) Development of thermally formed glass optics for astronomical hard x-ray telescopes. Optics Express, 7 (4). pp. 178-185. ISSN 1094-4087. http://resolver.caltech.edu/CaltechAUTHORS:CRAoe00
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The next major observational advance in hard X-ray/soft gamma-ray astrophysics will come with the implementation of telescopes capable of focusing 10-200 keV radiation. Focusing allows high signal-to-noise imaging and spectroscopic observations of many sources in this band for the first time. The recent development of depth-graded multilayer coatings has made the design of telescopes for this bandpass practical, however the ability to manufacture inexpensive substrates with appropriate surface quality and figure to achieve sub-arcminute performance has remained an elusive goal. In this paper, we report on new, thermally-formed glass micro-sheet optics capable of meeting the requirements of the next-generation of astronomical hard X-ray telescopes.
|Additional Information:||© 2000 Optical Society of America. Received June 22, 2000; Revised August 11, 2000. Measurements presented here were performed in part at the European Synchrotron Radiation Facility (ESRF). We wish to acknowledge A. Freund, E. Ziegler, R. Hustache, Manuel S. Del Rio, M. Ohler, and V. Honkimaki for their help with the ESRF portion of the measurements.|
|Group:||Space Radiation Laboratory|
|Subject Keywords:||OCIS codes: (340.0340) X-ray optics|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Archive Administrator|
|Deposited On:||18 May 2005|
|Last Modified:||08 Dec 2014 18:48|
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