The first demonstration of the concept of "narrow-FOV Si/CdTe semiconductor Compton camera"

The Soft Gamma-ray Detector (SGD), to be deployed onboard the {\it ASTRO-H} satellite, has been developed to provide the highest sensitivity observations of celestial sources in the energy band of 60-600~keV by employing a detector concept which uses a Compton camera whose field-of-view is restricte...

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Veröffentlicht in:	arXiv.org 2015-09
Hauptverfasser:	Ichinohe, Yuto, Uchida, Yuusuke, Watanabe, Shin, Edahiro, Ikumi, Hayashi, Katsuhiro, Kawano, Takafumi, Ohno, Masanori, Ohta, Masayuki, Takeda, Shin'ichiro, Fukazawa, Yasushi, Katsuragawa, Miho, Nakazawa, Kazuhiro, Odaka, Hirokazu, Tajima, Hiroyasu, Takahashi, Hiromitsu, Takahashi, Tadayuki, Yuasa, Takayuki
Format:	Artikel
Sprache:	eng
Schlagworte:	Background noise BGO (crystal) Field of view Gamma ray detectors Gamma rays Low temperature environments Physics - Instrumentation and Methods for Astrophysics Rejection Thermal vacuum tests Vacuum tests
Online-Zugang:	Volltext
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