S
S. Furui
Researcher at Hiroshima University
Publications - 8
Citations - 220
S. Furui is an academic researcher from Hiroshima University. The author has contributed to research in topics: Electron scattering & Scattering. The author has an hindex of 6, co-authored 8 publications receiving 191 citations.
Papers
More filters
Journal ArticleDOI
The Si/CdTe semiconductor Compton camera of the ASTRO-H Soft Gamma-ray Detector (SGD)
Shin Watanabe,Shin Watanabe,Hiroyasu Tajima,Yasushi Fukazawa,Yuto Ichinohe,Yuto Ichinohe,Shin'ichiro Takeda,Teruaki Enoto,Taro Fukuyama,Taro Fukuyama,S. Furui,Kei Genba,Kouichi Hagino,Kouichi Hagino,Atsushi Harayama,Yoshikatsu Kuroda,Daisuke Matsuura,Ryo Nakamura,Kazuhiro Nakazawa,Hirofumi Noda,Hirokazu Odaka,Masayuki Ohta,M. Onishi,Shinya Saito,Shinya Saito,G. Sato,Tamotsu Sato,Tamotsu Sato,Tadayuki Takahashi,Tadayuki Takahashi,Takaaki Tanaka,Atsushi Togo,Atsushi Togo,Shinji Tomizuka +33 more
TL;DR: The Soft Gamma-ray Detector (SGD) is one of the instrument payloads onboard ASTRO-H, and will cover a wide energy band (60-600) at a background level 10 times better than instruments currently in orbit.
Journal ArticleDOI
An x-ray spectral model of reprocessing by smooth and clumpy molecular tori in active galactic nuclei with the monaco framework
S. Furui,Yasushi Fukazawa,Hirokazu Odaka,Hirokazu Odaka,Toshihiro Kawaguchi,Masanori Ohno,K. Hayashi +6 more
TL;DR: In this article, an X-ray spectral model of reprocessing by a torus in an active galactic nucleus (AGN) with the Monte Carlo simulation framework MONACO is presented.
Journal ArticleDOI
X-ray Spectral Model of Reprocessing by Smooth and Clumpy Molecular Tori in Active Galactic Nuclei with the MONACO framework
TL;DR: In this article, an X-ray spectral model of reprocessing by a torus in an active galactic nucleus (AGN) with a Monte Carlo simulation framework was presented.
Journal ArticleDOI
Fe-K LINE TIME VARIABILITY AND Ni ABUNDANCE OF DISTANT REFLECTORS IN SEYFERT GALAXIES
TL;DR: In this article, the authors performed a systematic study of narrow Fe-K line (6.4 keV) flux variability and Ni-k line intensity for Seyfert galaxies.
Journal ArticleDOI
Fe-K Line Time variability and Ni abundance of Distant Reflector in Seyfert Galaxies
TL;DR: In this article, the authors performed a systematic study of narrow Fe-K line (6.4 keV) flux variability and Ni-k line intensity for Seyfert galaxies.