Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
The Tibet AS gamma Collaboration
The Tibet ASgamma Collaboration
Utsunomiya Univ., Japan
Osaka City University
Tokyo Univ., Tanashi, Japan
Saitama University
Kyoto University, Japan
Environment Sensing and Network Group, National Institute of Information and Communications Technology, Koganei, Japan
Saitama University, Urawa, Saitama, Japan
Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555, Japan; Saitama University, Saitama 338-8570, Japan
Department of Physics, Saitama University, Japan
Department of Physics, Saitama University, Urawa, Japan
Department of Physics, Saitama University, Saitama 338-8570, Japan; Advanced Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555, Japan
Communications Research Laboratory, Koganei, Tokyo, Japan
National Institute of Information and Communications Technology, Tokyo, Japan
Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555, Japan; Department of Physics, Saitama University, Saitama 338-8570, Japan
Department of Physics, Saitama University, Urawa 338-8570, Japan
Kyoto Univ., Japan
Kyoto University, Kyoto, Japan
National Institute of Information and Communications Technology, 4-2-1, Nukui- Kitamachi, Koganei, Tokyo, 184-8795, Japan Institute of Space and Astronautical Science
Department of Physics, Hirosaki University, Hirosaki, Japan
Saitama University, Saitama, Japan
Konan Univ., Kobe, Japan
Natioanl Institute of Information and Communication Technology, Koganei, Tokyo, Japan
Communications Research Laboratory, 4-2-1 Nukui-Kita Kogenai, Tokyo, 184-8795 Japan
Communications Research Laboratory, 4-2-1, Nukui-Kitamachi, Koganei, Tokyo, 184-8795 Japan
Department of Physics, Hirosaki University, Hirosaki, JapanZ.CaoL. K.DingInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing, ChinaZ. Y.FengDepartment of Physics, South West Jiaotong University, Chengdu, ChinaK.HibinoInstitute for Cosmic Ray Research, Universit
(C II) 158 micron and (O I) 63 micron observations of the Galactic center regions
3.3 micron emission feature in galaxies
3.3 micron emission feature in infrared galaxies
3.3-micron spectra of four IRAS sources
A forbidden C II 158-micron map of the M17 complex
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