Paper
29 September 1999 X-ray evolving universe spectroscopy mission (XEUS)
Marcos Bavdaz, Johan A.M. Bleeker, Gunther Hasinger, Hajime Inoue, Giorgio G.C. Palumbo, Anthony J. Peacock, Arvind N. Parmar, Martin J. L. Turner, Joachim E. Truemper, Jens Schiemann
Author Affiliations +
Abstract
XEUS: The X-ray Evolving Universe Spectroscopy mission represents a potential follow-on mission to the ESA XMM cornerstone currently nearing completion. XEUS represents the next logical step forward in x-ray astrophysics after the current set of mission have been launched and completed their operational lives. The development and ultimate success relies heavily on the capability of the International Space Station (ISS). In this paper we describe the key characteristics of the mission including the requirements placed specifically on the ISS and discuss the significant advances in high energy astrophysics expected from such an observatory.
© (1999) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Marcos Bavdaz, Johan A.M. Bleeker, Gunther Hasinger, Hajime Inoue, Giorgio G.C. Palumbo, Anthony J. Peacock, Arvind N. Parmar, Martin J. L. Turner, Joachim E. Truemper, and Jens Schiemann "X-ray evolving universe spectroscopy mission (XEUS)", Proc. SPIE 3766, X-Ray Optics, Instruments, and Missions II, (29 September 1999); https://doi.org/10.1117/12.363664
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Cited by 16 scholarly publications.
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KEYWORDS
Mirrors

X-rays

Space operations

Spectroscopy

Control systems

Astrophysics

Dye sensitized solar cells

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