Paper
8 October 2005 Sounding rocket payload development for x-ray observations of the Cygnus Loop
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Abstract
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 collimator 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.
© (2005) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Randall L. McEntaffer, Webster Cash, and Ann Shipley "Sounding rocket payload development for x-ray observations of the Cygnus Loop", Proc. SPIE 5900, Optics for EUV, X-Ray, and Gamma-Ray Astronomy II, 59001B (8 October 2005); https://doi.org/10.1117/12.615423
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Cited by 1 scholarly publication.
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KEYWORDS
Collimators

X-rays

Sensors

Diffraction gratings

Rockets

Ions

Clouds

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