Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
ISAS Japan, Japan
Institute of Astrophysics and Planetary Science, Ibaraki University, AL
Institute of Astrophysics and Planetary Science, Ibaraki University, Bunkyo, Mito, Ibaraki 310-8512
Institute of Astrophysics and Planetary Sciences, Ibaraki University, Mito, Ibaraki 310-8512 University, Mito, Ibaraki, Japan
Nobeyama Radio Observatory, Minamimaki, Japan
Institute of Space and Astronautical Science, JAXA, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510; Department of Astronomy, The University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033
Institute of Astrophysics and Planetary Science, Ibaraki University, 2-1-1 Bunkyo, Mito, Ibaraki, 310-8512, Japan
Institute of Astrophysics and Planetary Science, Ibaraki University, Bunkyo, Mito, Ibaraki, 310-8512 Japan
Nobeyama Radio Observatory, Minamisaku, Nagano, 384-1305, Japan
Nobeyama Radio Observatory, National Astronomical Observatory of Japan, Minamimaki, Minamisaku, Nagano 384-1305, Japan
Institute of Astrophysics and Planetary Science, Ibaraki University, Mito, Ibaraki 310
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510; Department of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033
Institute of Astrophysics and Planetary Science, Ibaraki University, Bunkyo, Mito, Ibaraki 310-8512; Nobeyama Radio Observatory, National Astronomical Observatory, Minamisaku, Nagano 384-1305
Institute of Space and Astronautial Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa, 229-8510, Japan
Institute of Space and Astronautical Science, Sagamihara, Kanagawa 252-5210, Japan; Department of Astronomy, The University of Tokyo, Bunkyo, Tokyo 113-0033, Japan
NAOJ & Graduate Univ. for Adv. Studies & Univ. Tokyo
Ibaraki Univ.
Natio
40- to 50-GHz array receiver with tunerless SIS mixers
87Sr/86Sr of apatite as an indicator of magma processes of the granites
A 32 m Parabolic Antenna in Peru At 3,370m of Altitude
A 45-m telescope with a surface accuracy of 65 μm.
A bright, dust-obscured, millimeter-selected galaxy beyond the Bullet Cluster (1E0657-56)
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