1 November 1990 Multilayer telescope for soft x-ray surveys
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The general design and performance characteristics of a 1-m diameter f/1.4 normal incidence X-ray Multilayer Telescope (XMT) operating at 0.13 keV are described. The principal scientific objectives of the XMT include soft diffuse X-rays, stellar surveys, interstellar dust grains, and soft excess in AGN. The feasibility of meeting these objectives using an XMT telescope is assessed.
© (1990) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Richard C. Catura, "Multilayer telescope for soft x-ray surveys", Proc. SPIE 1344, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy, (1 November 1990); doi: 10.1117/12.23269; https://doi.org/10.1117/12.23269


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