Paper
11 October 2004 New x-ray telescope mission (NeXT)
Author Affiliations +
Abstract
In various objects, it has been evident that non-thermal processes are playing important roles in high energy objects. They become outstanding above 10 keV and its total energy could be comparable to that of thermal components. In order to examine such non-thermal processes, we propose a hard X-ray imaging mission NeXT (New X-ray Telescope mission) together with the soft gamma ray detector and the high resolution spectrometer. Hard X-ray telescopes consist of multilayer coated high through put mirrors. The focal plane detectors are hybrid type imaging detectors to cover both soft and hard X-rays. Total performance in sensitivity for a point source reaches 100 times better than any currently scheduled missions in 10 - 60(80) keV range and 10 times better in soft gamma rays. It is planned to launch it in the time frame of 2011.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Hideyo Kunieda, Hajime Inoue, Kazuhisa Mitsuda, and Tadayuki Takahashi "New x-ray telescope mission (NeXT)", Proc. SPIE 5488, UV and Gamma-Ray Space Telescope Systems, (11 October 2004); https://doi.org/10.1117/12.550769
Lens.org Logo
CITATIONS
Cited by 3 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Hard x-rays

X-rays

Sensors

X-ray telescopes

Image sensors

Gamma radiation

X-ray imaging

RELATED CONTENT

High z gamma ray bursts for unraveling the dark ages...
Proceedings of SPIE (July 24 2014)
Swift: results from the first year of the mission
Proceedings of SPIE (July 26 2006)
New x-ray telescope mission (NeXT)
Proceedings of SPIE (January 29 2004)
Broadband x-ray imaging mission NeXT
Proceedings of SPIE (March 11 2003)

Back to Top