Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
National Astronomical Observatory of Japan, Tokyo, Japan
NAOJ
NAOJ Tokyo
National Astronomical Observatory, Japan
NAOJ, Japan
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan
National Astronomical Observatory, Tokyo, Japan
Subaru Telescope
National Astronomical Observatory, Osawa 2-21-1, Mitaka, Tokyo 181-8588, Japan.
Optical and Infrared Division and Extrasolar Planet Project Office, National Astronomical Observatory of Japan, Ōsawa 2-21-1, Mitaka-city, 181-8588 Tōkyō, Japan
National Astronomical Observatory of Japan, Japan
National Astronomical Observatory
NAO Japan
National Astronomical Observatory, Osawa 2-21-2, Mitaka, Tokyo 181, Japan
National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8858, Japan
National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan.
National Optical Astronomy Observatoires, Tucson, AZ
NAO, Japan
National Astronomical Observatory of Japan, Osawa, Mitaka, Tokyo 181-8588, Japan
National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588
National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
Division of Optical and Infrared Astronomy, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan
National Astronomical Observatory of Japan and The University of Electro-Communications
California Institute of Technology, Pasadena, CA, US
JPL, Pasadena, CA; Massachusetts, University, Amherst; National Optical Astronomy Observatoires, Tucson, AZ
National Astronomical Observatory of Japan, Osawa, Mitaka, Tokyo 181-8588, Japan Radio Observatory, Japan
Gemini Observatory, Hawaii, USA
Optical and Infrar
$^{13}$C NMR Study on Zero-Gap State in the Organic Conductor $θ$-(BEDT-TTF)$_{2}$I$_{3}$ under Pressure
2 Millimeter Observations of Bright-rimmed Clouds with IRAS Point Sources
A 400-3500 nm spectroscopy through a common-path interfero coronagraph instrument on 600 mm telescope on RS ISS
A coronagraph system with unbalanced nulling interferometer and fourth-order coronagraphs
A Coronagraph with an Unbalanced Nulling Interferometer and Adaptive Optics
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