Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
University of Tokyo
Faculty of Education, Saitama University, 255 Shimo-Okubo, Sakura, Saitama 338-8570
Kobe University, Japan School of Science and Technology, Kobe University, 1-1 Rokkodai, Nada-ku, Kobe 657-8501
Graduate School of Science, Kobe University, 1-1 Rokkodai, Nada, Kobe, Hyogo 657-8501, Japan
National Space Development Agency of Japan
Earth Observation Research Center, National Space Development Agency of Japan
Graduate School of Science, Kobe University, 1-1 Rokkodai, Nada, Kobe 657-8501; Department of Education, Saitama University, 255 Shimo-Okubo, Sakura-ku, Saitama 338-8570
Department of Astronomy, University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
Graduate School of Science and Technology, Kobe University, 1-1 Rokkodai, Nada, Kobe, Hyogo 657-8501, Japan.
Graduate School of Science and Technology, Kobe University, 1-1 Rokkodai, Nada-ku, Kobe 657-8501, Japan.
Graduate School of Science, Kobe University, 1-1 Rokkodai, Nada-ku, Kobe 657-8501
Graduate School of Science, Kobe University, 1-1 Rokkodai-cho, Nada-ku, Kobe, Hyogo 657-8501
Earth Observation Research Center, National Space Development Agency of Japan, 1-8-10 Harumi, Chuo-ku, Tokyo 104-6023, Japan
National Space Development Agency of Japan / Earth Observation Research Center, Harumi Island Triton Square Office Tower X 23F, 1-8-10, Harumi, Chuo-ku, Tokyo 104-6023, Japan
University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
Graduate School of Science and Technology, Kobe University, 1-1, Rokkodai, Nada, Kobe, Hyogo 657-8501, Japan
NASDA, Japan
Department of Astronomy, University of Tokyo, Japan
NASDA, Harumi, Chuo-ku, Tokyo 104-6023, Japan
A coronagraphic search for brown dwarfs and planets around nearby stars
A Deep Near Infrared Imaging Survey of the Lupus 3 Dark Cloud
A Deep Near-Infrared Survey of the Chamaeleon I Dark Cloud Core
A Near-Infrared Imaging Survey of the Lupus 3 Dark Cloud: A Modest Cluster of Low-Mass, Pre-Main-Sequence Stars
A Spectroscopic Confirmation of of Young Brown Dwarfs and Planetary-Mass Objects
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