L. Pina,1 R. Hudec,1,2 V. Tichy,1 A. Inneman,3 D. Cerna,3 L. Sveda,1 J. Marsik,3 V. Marsikova,3 W. Cash,4 A. F. Shipley,4 B. R. Zeiger,4 T. D. Rogers4
1Czech Technical Univ. in Prague (Czech Republic) 2Astronomical Institute, Academy of Sciences of the ASCR, v.v.i. (Czech Republic) 3Rigaku Innovative Technologies Europe (Czech Republic) 4Univ. of Colorado at Boulder (United States)
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A novel design of X-ray optical system - concentrator for astrophysical rocket experiment is investigated. The proposed system is
based on four modules with Kirkpatrick-Baez (KB) configuration allowing usage of multi-foil mirrors arranged to parabolic profile.
The KB modules are supplemented by rotationally symmetrical parabolic segments. This X-ray optical system effectively uses
a circular aperture. The KB modules are placed in four quadrants while the segments are set into a Cartesian cross between
the KB modules. Studied optical system is under consideration for the student rocket experiment of University of Colorado that
should verify function of NIST’s energy-dispersive detector based on Transition Edge Sensors (TES microcalorimeters).
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L. Pina, R. Hudec, V. Tichy, A. Inneman, D. Cerna, L. Sveda, J. Marsik, V. Marsikova, W. Cash, A. F. Shipley, B. R. Zeiger, T. D. Rogers, "Design of novel x-ray optical system for rocket experiment," Proc. SPIE 8848, Advances in X-Ray/EUV Optics and Components VIII, 884805 (27 September 2013); https://doi.org/10.1117/12.2023984