Hiroshima University / Kogakuin University / University of Tokyo / Kyoto University / Rikkyo University / Nagoya University / Ehime University / Aoyama Gakuin University / Tokyo Institute of Technology / Kanazawa University / Osaka University / Saitama University / /
IndustryTerm
high-energy non-thermal phenomena / high energy instruments / high energy response / non-imaging instruments / power-law spectrum / high energy resolution / high-energy universe / possible solution / energy range / connection technology / accelerated high energy particles / high-energy non-thermal universe / pixels active area energy resolution / energy resolution / imaging / energy content / wide energy range / wide energy band / active area energy resolution pixel size thickness number / energy / /
MusicGroup
X-ray / Gamma / /
Organization
ASIC / Stanford Linear Accelerator Center / Astro-E2 mission / Ehime University / NeXT mission / Kanazawa University / Nagoya University / US Federal Reserve / Aoyama Gakuin University / Kyoto University / Hiroshima University / Saitama University / University of Tokyo / National Aeronautics and Space Administration / Japanese MAXI mission / Institute of Space and Astronautical Science / Department of Physics / Rikkyo University / Tokyo Institute of Technology / Kogakuin University / Stanford / Osaka University / /
Wide band X-ray Imager (WXI) and Soft Gamma-ray Detector (SGD) for the NeXT Mission T. Takahashia,b , A. Awakic , T. Dotania , Y. Fukazawad , K. Hayashidae , T. Kamaef , J. Kataokag , N. Kawaig , S. Kitamotoh , T. Kohmur