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Dive into the research topics where Tadahisa Tamura is active.

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Featured researches published by Tadahisa Tamura.


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1990

Use of a large area photodiode in CsI(Tl) scintillation counters

Shuichi Gunji; N. Hanada; T. Hoshino; T. Kamae; S. Miyazaki; T. Takahashi; Tadahisa Tamura; M. Tanaka; Takamasa Yamagami; H. Murakami; K. Mori; Hitoshi Tanaka; K. Yamamoto

Abstract A newly developed large area photodiode has been studied as the photon sensor for medium-size CsI(Tl) scintillation counters. The photodiode has a sensitive area of 18 × 18 mm 2 and a thickness of 500 μm. When combined with a CsI(Tl) crystal of 2.5 × 2.5 × 5.0 cm 3 , it gives an energy resolution of around 5.1% (FWHM) for 1.33 MeV gamma-rays. Characteristics of the low noise preamplifier designed for the CsI(Tl)-photodiode counter will also be given.


COMPTON GAMMA‐RAY OBSERVATORY | 1993

Hard x‐ray observation of Cen A and a break in the energy spectrum

T. Takahashi; Shuichi Gunji; M. Hirayama; T. Kamae; S. Miyazaki; Yutaro Sekimoto; M. Tanaka; Tadahisa Tamura; Noriko Y. Yamasaki; H. Inoue; T. Kanou; T. Yamagami; M. Nomachi; H. Murakami; J. Braga; J. A. Neri

We studied hard X‐ray/γ‐ray emission from Cen A (NGC 5128) in a balloon experiment with a low background detector (Welcome‐1) in Brazil. The energy spectrum of CenA is obtained from 40 keV to 600 keV. We combined the energy spectrum obtained by the Ginga satellite in a similar state. The combined spectrum indicates that there is a break at 185±22 keV. The spectrum is fitted to the broken power law model with the photon index of α1=−1.79 up to 188 keV, and α2=−3.7−1.7+0.9 above the break.


Advances in Space Research | 1993

Detector to study low-flux hard X-ray/gamma-ray sources

T. Kamae; T. Takahashi; M. Tanaka; Shuichi Gunji; S. Miyazaki; Tadahisa Tamura; Yutaro Sekimoto; N. Yamaoka; J. Nishimura; N. Yajima; Takamasa Yamagami; M. Nomachi; H. Murakami; M. Nakagawa; A. Neri

Abstract We have developed a new kind of phoswich counters that will be capable of detecting low flux hard X-rays/gamma-rays from astronomical objects. The new phoswich counter consists of a small inorganic scintillator with a fast decay time (the detection part) glued to the interior bottom surface of a rectangular well-shaped block of another inorganic scintillator with a slow decay time (the shielding part). Here, the well-shaped shielding part acts as an active collimator as well as an active shield. We have built a detector system consisting of 64 such phoswich counters: newly developed scintillator (GSO) is used for the detection part and CsI( Tl ) is used for the shielding part. The total geometrical area of the 64 detection parts is about 740cm 2 and its 3σ sensitivity is expected to reach below 10 −5 cm −2 s −1 keV −1 up to 700keV. With several improvements such detectors will be able to detect hard X-rays/gamma-rays at a flux level around 10 −6 cm −2 s −1 keV −1 upto 2 MeV.


Publications of the Astronomical Society of Japan | 1996

X- Ray/Soft Gamma-Ray Observation of Centaurus A and Its Implication on the Emission Mechanism

Satoshi Miyazaki; Tadayuki Takahashi; Shuichi Gunji; M. Hirayama; Tuneyoshi Kamae; Yutaro Sekimoto; Tadahisa Tamura; M. Tanaka; Noriko Y. Yamasaki; Hajime Inoue; Takako Kano; Takamasa Yamagami; M. Nomachi; Hiroyuki Murakami; John Braga; J. Angelo Neri


宇宙科学研究所報告. 特集 | 1998

Diffusive Reacceleration of Cosmic Ray Electrons in the Galaxy

Y. Komori; Jun Nishimura; T. Kobayashi; S. Torii; Takamasa Yamagami; K. Yoshida; Tadahisa Tamura


Archive | 2016

In-flight Performance and First Results of CALET Gamma-ray Burst Monitor

貴紀 坂本; 篤正 吉田; 一郎 高橋; 雄太 川久保; 一真 瀬沼; 光明 森山; 祐介 山田; 和貴 山岡; 聡志 中平; 陽一 浅岡; 俊介 小澤; 祥二 鳥居; 雄輝 清水; 忠久 田村; マイク チェリー; セルジオ リッカリーニ; ピエール マロチェシー; Takanori Sakamoto; Atsumasa Yoshida; Ichiro Takahashi; Y. Kawakubo; Kazumasa Senuma; Mitsuaki Moriyama; Yusuke Yamada; Kazutaka Yamaoka; Youichi Asaoka; S. Ozawa; S. Torii; Y. Shimizu; Tadahisa Tamura


Meeting abstracts of the Physical Society of Japan | 2014

28aTS-5 CALET Telemetory Data Simulation on ISS Orbit

Kenta Shimomura; S. Torii; Y. Asaoka; S. Ozawa; Katsuaki Kasahara; Yasuki Kamio; Tae Niita; Holger Motz; Kazuki Rikiishi; Tadahisa Tamura; Shiro Ueno; Y. Shimizu; Hiroshi Tomida; Yosui Akaike


Archive | 2010

CALET investigation of the origin of cosmic-ray electrons and search for dark matter

Kenji Yoshida; S. Torii; Kazuo Kasahara; Yosui Akaike; Tadahisa Tamura; Masaki Mori; Kunihito Ioka; Norita Kawanaka


Archive | 2008

Design and Performance of Balloon-borne CALET Prototype Detector

Yasuhiro Fukuta; S. Torii; Kazuo Kasahara; Y. Shimizu; Yosui Akaike; K. Taira; Ken Hidaka; Tadahisa Tamura; Y. Katayose; H. Murakami


Archive | 2008

bCALET-2による高エネルギー電子・ガンマ線観測計画

忠久 田村; Tadahisa Tamura; 欣也 日比野; K. Hibino; 祥二 奥野; S. Okuno; 祥二 鳥居; S. Torii; 克昌 笠原; Katsuaki Kasahara; 俊介 小澤; S. Ozawa; 慈治 有働; S. Udo; 陽水 赤池; Yosui Akaike; 晃一 平; K. Taira; 健 日高; Ken Hidaka; 康博 福田; Yasuhiro Fukuda; 浩之 村上; H. Murakami; 隆正 山上; Takamasa Yamagami; 芳隆 斎藤; Y. Saito; 英之 福家; Hideyuki Fuke

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K. Yoshida

Shibaura Institute of Technology

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