Paper
28 November 2000 Evaluation and optimization of multilayer designs for astronomical x-ray telescopes using a field-of-view- and energy-dependent figure of merit
Peter H. Mao, Leon M. Bellan, Fiona A. Harrison, David L. Windt, Finn Erland Christensen
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Abstract
The three most important quantities used to assess the performance of astronomical x-ray telescope optics are the on- axis collecting area, the field of view, and the half-power diameter. The first two quantities depend on the mirror packing arrangement and the multilayer coating design. In order to optimize the coating design, we have developed a figure-of-merit (FOM) that accounts for the coating response over a specified range of energies and off-axis angles. We present an example where we have used this FOM to optimize a specific coating design for the High Energy Focusing Telescope (HEFT) and to understand tradeoffs between performance and coating thickness.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Peter H. Mao, Leon M. Bellan, Fiona A. Harrison, David L. Windt, and Finn Erland Christensen "Evaluation and optimization of multilayer designs for astronomical x-ray telescopes using a field-of-view- and energy-dependent figure of merit", Proc. SPIE 4138, X-Ray Optics, Instruments, and Missions IV, (28 November 2000); https://doi.org/10.1117/12.407561
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Cited by 3 scholarly publications.
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KEYWORDS
Mirrors

Coating

Multilayers

Telescopes

Optical instrument design

X-ray telescopes

Reflectivity

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