Sebastian Diebold, Josef Jochum, Eckhard Kendziorra, Emanuele Perinati, Andrea Santangelo, Chris Tenzer
Kepler Center for Astro and Particle Physics, Universität Tübingen
To be published in: Proceedings of the RADECS 2013
Abstract. Orbital soft protons (from tens of keV to a few MeV) can seriously degrade the performance of astronomical X-ray detectors. This paper briefly describes an irradiation setup for large detectors at the accelerator facility of the University of Tübingen. Main advantages are a high flux uniformity over a large area as well as a precise monitoring system for the applied spectrum and fluence. Recent modifications of this setup that enable measurements of the small angle scattering efficiency of Wolter-type X-ray mirror shells are presented.
Preprint (1,53 Mb PDF file including figures)
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Last modified 12 Nov 2013 |