Paper
18 July 2000 The evolving universe spectroscopy mission (XEUS)
Marcos Bavdaz, Anthony J. Peacock, Arvind N. Parmar, Marco W. Beijersbergen, Jens Schiemann
Author Affiliations +
Abstract
The X-ray Evolving Universe Spectroscopy mission (XEUS) is a potential follow-on to ESA's Cornerstone XMM-Newton. XEUS is designed to become a permanent space-based X-ray observatory covering the waveband from 0.5 to 200 angstroms with a sensitivity comparable to the most advanced planned future observations at longer wavelengths, such as NGST, ALMA and FIRST.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Marcos Bavdaz, Anthony J. Peacock, Arvind N. Parmar, Marco W. Beijersbergen, and Jens Schiemann "The evolving universe spectroscopy mission (XEUS)", Proc. SPIE 4012, X-Ray Optics, Instruments, and Missions III, (18 July 2000); https://doi.org/10.1117/12.391567
Lens.org Logo
CITATIONS
Cited by 2 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Mirrors

X-rays

Spectroscopy

Space operations

Observatories

Sensors

X-ray optics

RELATED CONTENT

DIOS: the dark baryon exploring mission
Proceedings of SPIE (July 25 2014)
The NASA X-ray Mission concepts study
Proceedings of SPIE (September 17 2012)
Kirkpatrick-Baez optics for the Generation-X mission
Proceedings of SPIE (October 07 2005)
Status of the optics for the X ray Evolving Universe...
Proceedings of SPIE (November 28 2000)

Back to Top