647 citations · 5.8k across the 112 of their papers we have counts for
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phi photo-production from Li, C, Al, and Cu nuclei at Egamma=1.5 - 2.4 GeV
T. Ishikawa, D. S. Ahn, J. K. Ahn +39
The photo-production of mesons from Li, C, Al, and Cu at forward angles has been measured at =1.5--2.4 GeV. The number of events for incoherent phi photo-production is…
Wide band X-ray Imager (WXI) and Soft Gamma-ray Detector (SGD) for the NeXT Mission
T. Takahashi, A. Awaki, T. Dotani +25
The NeXT mission has been proposed to study high-energy non-thermal phenomena in the universe. The high-energy response of the super mirror will enable us to perform the first sens…
A Prototype Si/CdTe Compton Camera and the Polarization Measurement
Takefumi Mitani, Takaaki Tanaka, Kazuhiro Nakazawa +7
A Compton camera is the most promising approach for gamma-ray detection in the energy region from several hundred keV to MeV, especially for application in high energy astrophysics…
Development of a Si/CdTe semiconductor Compton telescope
Takaaki Tanaka, Takefumi Mitani, Shin Watanabe +10
We are developing a Compton telescope based on high resolution Si and CdTe imaging devices in order to obtain a high sensitivity astrophysical observation in sub-MeV gamma-ray regi…
Gamma-ray Polarimetry with Compton Telescope
Hiroyasu Tajima, Grzegorz Madejski, Takefumi Mitani +10
Compton telescope is a promising technology to achieve very high sensitivity in the soft gamma-ray band (0.1-10 MeV) by utilizing Compton kinematics. Compton kinematics also enable…
The Majorana Neutrinoless Double-Beta Decay Experiment
Aalseth
The proposed Majorana double-beta decay experiment is based on an array of segmented intrinsic Ge detectors with a total mass of 500 kg of Ge isotopically enriched to 86% in 76Ge.…
Performance of a Low Noise Front-end ASIC for Si/CdTe Detectors in Compton Gamma-ray Telescope
H. Tajima, T. Nakamoto, T. Tanaka +11
Compton telescopes based on semiconductor technologies are being developed to explore the gamma-ray universe in an energy band 0.1--20 MeV, which is not well covered by the present…