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The NeXT Mission

Authors :
Y. Ogasaka
Hiroshi Tsunemi
Kiyoshi Hayashida
H. Tajima
Kazuhisa Mitsuda
G. M. Madejski
Ryuichi Fujimoto
Shin Watanabe
Yukikatsu Terada
Kazuo Makishima
Katsuji Koyama
Motohide Kokubun
Kazuhiro Nakazawa
Takeshi Go Tsuru
K. Mori
Y. Ishisaki
Yoshihiro Ueda
Yasushi Fukazawa
N. E. White
M. Ozaki
Manabu Ishida
Robert Petre
Tadayasu Dotani
R. F. Mushotzky
Tadayuki Takahashi
Makoto Tashiro
Takaya Ohashi
Hideyo Kunieda
Noriko Y. Yamasaki
NeXT team
R. L. Kelley
Source :
Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray.
Publication Year :
2008
Publisher :
SPIE, 2008.

Abstract

The NeXT (New exploration X-ray Telescope), the new Japanese X-ray Astronomy Satellite following Suzaku, is an international X-ray mission which is currently planed for launch in 2013. NeXT is a combination of wide band X-ray spectroscopy (3 - 80 keV) provided by multi-layer coating, focusing hard X-ray mirrors and hard X-ray imaging detectors, and high energy-resolution soft X-ray spectroscopy (0.3 - 10 keV) provided by thin-foil X-ray optics and a micro-calorimeter array. The mission will also carry an X-ray CCD camera as a focal plane detector for a soft X-ray telescope and a non-focusing soft gamma-ray detector. With these instruments, NeXT covers very wide energy range from 0.3 keV to 600 keV. The micro-calorimeter system will be developed by international collaboration lead by ISAS/JAXA and NASA. The simultaneous broad bandpass, coupled with high spectral resolution of Delta E ~ 7 eV by the micro-calorimeter will enable a wide variety of important science themes to be pursued.<br />14 pages, 10 figures, Proceedings of the SPIE meeting, "Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray 2008", Marseille (2008)

Details

ISSN :
0277786X
Database :
OpenAIRE
Journal :
Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray
Accession number :
edsair.doi.dedup.....e68dc1c9ce28a231b096d32d618cb89e
Full Text :
https://doi.org/10.1117/12.789640