Physics – Condensed Matter – Strongly Correlated Electrons
Scientist
Physics
Condensed Matter
Strongly Correlated Electrons
Scientist
ISAS, Sagamihara, Kanagawa, Japan
Institute for Solid State Physics, Tokyo University, Japan
Kyoto;
ISSP
BNL
University of Kyoto
Institute for Solid State Physics, The University of Tokyo, Tokyo, Japan
Kyoto Univ
ISSP, University of Tokyo
Institute for Solid State Physics, University of Tokyo, Japan
The Institute of Space and Astronautical Science
Kure National College of Technology
ISAS
Kyoto University, Japan
Institute of Space and Astronautical Science, Kanagawa 229-8510, Japan Yoshinodai 3-1-1, Sagamihara, Kanagawa 229, Japan
Japan Coast Guard Academy, 5-1 Wakaba-cho, Kure-si, Hiroshima 737-0832, Japan
Institute of Space and Astronautical Science, Sagamihara, 229-8510, Japan
Institute of Space and Astronautical Science, Yoshinodai 3-1-1, Sagamihara, Kanagawa 229-8510, Japan; Department of Astronomy, Kyoto University, Kyoto 606-8502, Japan.
Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan.
Department of Electrical Engineering, University of Tokyo, Tokyo 113-8656, Japan
Max-Planck-Institut für extraterrestrische Physik, D-85748 Garching bei München, Germany
High-Energy Astrophysics Division, ISAS, Kanagawa 229-8510, Japan
Kanazawa University, Kakuma, Kanazawa, Ishikawa 920-1192, Japan
RASC, Kyoto University, Gokasho, Uji, Kyoto, 611-0011 Japan
University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan.
Department of Astronomy, Kyoto Univ., Sakyo, Kyoto 606-8502
Japan Coast Guard Academy, 5-1, Wakaba-cho, Kure-shi, Hiroshima, Japan
Institute of Space and Astronautical Science, Yoshinodai 3-1-1 Sagamihara, Kanagawa 229-8510, Japan
Institute of Space and Astronautical Science Sagamihara, Kanagawa 229-8510, Japan
Institute of Space and Astronautical Science, 3-1-1, Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
A giant flare from a weak-lined T Tauri Star TWA-7 detected with MAXI/GSC
A new instrument for the study of wave-particle interactions in space: One-chip Wave-Particle Interaction Analyzer
A New Scheme for Estimating the Degree of Space Weathering Through Visible Multiband Spectroscopy Using an ECAS-Type Filter System Such as Hayabusa AMICA
A Pilot Survey for KX QSOs in the UKIDSS Ultra Deep Survey Field
A population of faint galaxies that contribute to the cosmic X-ray background
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