Wide band X-ray Imager (WXI) and Soft Gamma-ray Detector (SGD) for the NeXT Mission
Author(s) -
Tadayuki Takahashi,
A. Awaki,
Tadayasu Dotani,
Yasushi Fukazawa,
Kiyoshi Hayashida,
T. Kamae,
J. Kataoka,
N. Kawai,
Shunji Kitamoto,
Takayoshi Kohmura,
M. Kokubun,
Katsuji Koyama,
Kazuo Makishima,
Hironori Matsumoto,
Emi Miyata,
T. Murakami,
K. Nakazawa,
M. Nomachi,
Masanobu Ozaki,
H. Tajima,
M. Tashiro,
Toru Tamagawa,
Y. Terada,
H. Tsunemi,
Takeshi Go Tsuru,
K. Yamaoka,
Daisuke Yonetoku,
A. Yoshida
Publication year - 2004
Publication title -
proceedings of spie, the international society for optical engineering/proceedings of spie
Language(s) - English
Resource type - Conference proceedings
eISSN - 1996-756X
pISSN - 0277-786X
DOI - 10.1117/12.551500
Subject(s) - physics , detector , photon , gamma ray , optics , spectral line , telescope , nuclear physics , astronomy
The NeXT mission has been proposed to study high-energy non-thermal phenomenain the universe. The high-energy response of the super mirror will enable us toperform the first sensitive imaging observations up to 80 keV. The focal planedetector, which combines a fully depleted X-ray CCD and a pixellated CdTedetector, will provide spectra and images in the wide energy range from 0.5 keVto 80 keV. In the soft gamma-ray band up to ~1 MeV, a narrow field-of-viewCompton gamma-ray telescope utilizing several tens of layers of thin Si or CdTedetector will provide precise spectra with much higher sensitivity than presentinstruments. The continuum sensitivity will reach several times 10^(-8)photons/s/keV/cm^(2) in the hard X-ray region and a few times10^(-7)photons/s/keV/cm^(2) in the soft gamma-ray region.Comment: 12 pages, 13 figures, to be published in the SPIE proceedings 5488, typo corrected in sec.
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