A multilayer telescope for soft X-ray surveys

Details A multilayer telescope for soft X-ray surveys A multilayer telescope for soft X-ray surveys

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990spie.1344..438c&link_type=abstract

IN: EUV, X-ray, and Gamma-ray instrumentation for astronomy; Proceedings of the Meeting, San Diego, CA, July 11-13, 1990 (A92-20

Astronomy and Astrophysics

Astronomy

Spaceborne Telescopes, X Ray Astronomy, X Ray Telescopes, Active Galactic Nuclei, Cosmic Dust, Design Analysis

Scientific paper

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.

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