Paper
15 July 2008 Hard x-ray imaging system for XEUS
Author Affiliations +
Abstract
One of the major sciences of XEUS is the evolution of massive black holes from early to current Universe. As is well known, considerable fraction of massive black holes harbored in active galactic nuclei are embedded in thick absorbing material. In order to observe black holes without any bias of absorption, we propose a hard X-ray imaging system to XEUS. The hard X-ray imaging system is consisted of super mirror X-ray telescopes with multilayer coating and of the position sensitive hard X-ray imaging CdTe detector. Under the current boundary conditions, the design parameters will be optimized for the telescope and the multilayers. Current achievements of hard X-ray imaging detectors are also presented.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Hideyo Kunieda, Tadayuki Takahashi, Motohide Kokubun, Kazuhiro Nakazawa, and Yasushi Ogasaka "Hard x-ray imaging system for XEUS", Proc. SPIE 7011, Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray, 70110D (15 July 2008); https://doi.org/10.1117/12.787421
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Hard x-rays

Sensors

Imaging systems

X-rays

Silicon

X-ray telescopes

Absorption

RELATED CONTENT

The Hard X ray Imager (HXI) for the ASTRO H...
Proceedings of SPIE (September 17 2012)
ROSITA: scientific goal and mission concept
Proceedings of SPIE (March 11 2003)
Broadband x-ray imaging mission NeXT
Proceedings of SPIE (March 11 2003)
Hard x-ray imager (HXI) for the ASTRO-H Mission
Proceedings of SPIE (July 29 2010)
Next-generation x-ray observatory
Proceedings of SPIE (September 01 1995)

Back to Top