11 October 2004 High-resolution x-ray spectroscopy of supernova remnants and the diffuse background
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We present progress in the development of a new sounding rocket payload that will perform high resolution (R~100) x-ray spectroscopy of diffuse celestial x-ray sources. The instrument features a new geometry that allows for high resolution along with high throughput. A wire-grid focuser constrains light from diffuse sources into a converging beam that feeds an array of diffraction gratings in the extreme off-plane mount. Starting with launch in 2006 we can obtain physical diagnostics of supernova remnants such as the Cygnus Loop and ultimately the hot phase of the interstellar medium.
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Randall L. McEntaffer, Randall L. McEntaffer, Webster C. Cash, Webster C. Cash, } "High-resolution x-ray spectroscopy of supernova remnants and the diffuse background", Proc. SPIE 5488, UV and Gamma-Ray Space Telescope Systems, (11 October 2004); doi: 10.1117/12.552847; https://doi.org/10.1117/12.552847


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