Paper
11 November 1994 High-resolution x-ray spectroscopy with a rocket-borne cosmic x-ray microcalorimeter spectrograph
Arthur B. C. Walker II, Aharon Kapitulnik, Richard B. Hoover, Lawrence Lesyna, Melville P. Ulmer
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Abstract
The x-ray microcalorimeter represents a revolutionary development in x-ray astronomy, because it permits spectra to be obtained which rival Bragg crystal spectra in resolution, and exceed a proportional counter in efficiency. We describe a rocket borne x-ray spectrograph, consisting of a microcalorimeter detector array placed at the focus of a Wolter I collector. We demonstrate that a modest collecting area of 60 cm2 is sufficient to determine the abundances of O, Ne and Fe in the interstellar medium.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Arthur B. C. Walker II, Aharon Kapitulnik, Richard B. Hoover, Lawrence Lesyna, and Melville P. Ulmer "High-resolution x-ray spectroscopy with a rocket-borne cosmic x-ray microcalorimeter spectrograph", Proc. SPIE 2279, Advances in Multilayer and Grazing Incidence X-Ray/EUV/FUV Optics, (11 November 1994); https://doi.org/10.1117/12.193129
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KEYWORDS
X-rays

Spectrographs

Mirrors

Rockets

Spectroscopy

Hydrogen

Silicon

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