Paper
11 March 2003 Development and production of hard X-ray multilayer optics for HEFT
Jason E. Koglin, Finn Erland Christensen, Jim Chonko, William W. Craig, Todd R. Decker, Mario A. Jimenez-Garate, Kurt S. Gunderson, Charles J. Hailey, Fiona A. Harrison, Carsten P. Jensen, Mike Sileo, David L. Windt, Haitao Yu
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Abstract
The High Energy Focusing Telescope (HEFT) 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 mirrors that form these layers are made of thermally formed glass substrates coated with depth-graded multilayer films for enhanced reflectivity. The mirrors are assembled using an over-constraint method that forces the overall shape of the nominally cylindrical substrates to the appropriate conic form. We will present performance data on the HEFT optics and report the current status of the assembly production.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jason E. Koglin, Finn Erland Christensen, Jim Chonko, William W. Craig, Todd R. Decker, Mario A. Jimenez-Garate, Kurt S. Gunderson, Charles J. Hailey, Fiona A. Harrison, Carsten P. Jensen, Mike Sileo, David L. Windt, and Haitao Yu "Development and production of hard X-ray multilayer optics for HEFT", Proc. SPIE 4851, X-Ray and Gamma-Ray Telescopes and Instruments for Astronomy, (11 March 2003); https://doi.org/10.1117/12.461479
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Cited by 14 scholarly publications.
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KEYWORDS
Glasses

Mirrors

Metrology

X-ray optics

X-rays

Ultraviolet radiation

Multilayers

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