Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Galaxy Astrophysics
Scientist
DIAS
ISAS / JAXA Jp
Kyoto Univ.
RIKEN
Riken, Japan
Kyoto University
RIKEN, Japan
ISAS / JAXA, Japan
Kyoto Unibersity
ISAS / JAXA, Yoshinodai, 3-1-1, Sagamihara, Kanagawa, Japan
Institute of Space and Astronautical Science, JAXA, Yoshinodai, Sagamihara, Kanagawa 229-8510
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510
School of Cosmic Physics, Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland Institute of Space and Astronautical Science / JAXA, 3-1-1 Yoshinodai, Chuo, Sagamihara 252-5210
Cosmic Radiation Laboratory, RIKEN, 2-1 Hirosawa, Wako, Saitama 351-0198
Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510
ISAS Japan, Japan
Kyoto University, Kyoto, Japan
School of Cosmic Physics, DIAS, 31 Fitzwilliam Place, Dublin 2, Ireland and ISAS / JAXA, 3-1-1 Yoshinodai, Sagamihara, Kanagawa, 229-8510, Japan
Kyoto Univ. Japan
RIKEN Cosmic Radiation Group, 2-1, Hirosawa, Wako-shi, Saitama, Japan of Physics, Kyoto University, Sakyo-ku, Kyoto 606-8502, Japan
Department of Physics, Faculty of Science, Kyoto University, Kitashirakawa-Oiwake-cho, Sakyo-ku, Kyoto, 606-8502, Japan 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
Institute of Space and Astronautical Science, JAXA, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
Department of Physics, Kyoto University, Kitashirakawa, Sakyo, Kyoto 606-8502, Japan
A Chandra Deep X-ray Exposure on the Galactic Plane and Near Infrared Identification
A Detailed Observation of a LMC Supernova Remnant DEM L241 with XMM-Newton
A Detailed Spatial and Spectral Study of Synchrotron X-rays from Supernova Remnants with Chandra
A Diffuse X-Ray Source, AX J1843.8-0352: Association with the Radio Complex G28.6-0.1 and Identification of a New Supernova Remnant
A hybrid X-ray imaging spectrometer for NeXT and the next generation X-ray satellite
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