Physics
Optics
Scientist
Key Laboratory for Research in Galaxies and Cosmology, SHAO, CAS, China;
The Institute of Space and Astronautical Science
Shangai Astronomical Observatory, China
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030
National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588
National Astronomical Observatory, Mitaka, Tokyo 181-8588
Shanghai Astronomical Observatory, Shanghai 200030
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030; Joint Institute for Galaxy and Cosmology
Shanghai Observatory, Chinese Academy of Sciences, Shanghai 200030
Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, P.R. China; Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, JAXA, Yoshinodai 3-1-1, Sagamihara, Kanagawa 229-8510; National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588
Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai, 200030, China
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China; Joint Institute for Galaxy and Cosmology, ShAO and USTC, Chinese Academy of Sciences, China
Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, P.R.China
Shanghai Astronomical Observatory, 80 Nandan Road, Shanghai 200030, China
Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China; Joint Institute for Galaxy and Cosmology, Shanghai Astronomical Observatory and University of Science & Technology of China, China
Netherlands Foundation for Research in Astronomy, the Netherlands; L.I. Matveyenko Institute for Space Research, Moscow, Russia
Nanjing University, People's Republic of China
Department of Astrono
3 mm line survey towards a new sample of massive young stellar objets: GLIMPSE-identified EGOs
3C 84 Expanding Radio Lobe Revealed by VSOP Observations
7 mm VLBA Observations of Quasar OV-236
95GHz methanol maser survey toward GLIMPSE EGOs (Chen+, 2011)
A 5 GHz Southern Hemisphere VLBI Survey of Compact Radio SOurces - I
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