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Subo Dong

Researcher at Peking University

Publications -  334
Citations -  18263

Subo Dong is an academic researcher from Peking University. The author has contributed to research in topics: Gravitational microlensing & Light curve. The author has an hindex of 71, co-authored 318 publications receiving 16344 citations. Previous affiliations of Subo Dong include Princeton University & Ohio State University.

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Discovery and mass measurements of a cold, 10 earth mass planet and its host star

Yasushi Muraki, +129 more
TL;DR: In this article, the discovery and mass measurement of the cold, low-mass planet MOA-2009-BLG-266Lb, made with the gravitational microlensing method, is presented.
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Thirty Meter Telescope Detailed Science Case: 2015

Warren Skidmore, +142 more
TL;DR: The TMT Detailed Science Case describes the transformational science that the Thirty Meter Telescope (TMT) will enable as mentioned in this paper, and more than 150 astronomers from within the TMT partnership and beyond offered input in compiling the new 2015 detailed science case, including the California Institute of Technology (Caltech), the Indian Institute of Astrophysics (IIA), the National Astronomical Observatories of the Chinese Academy of Sciences (NAOC), the NaOJ, the University of California, the Association of Canadian Universities for Research in Astronomy (ACURA) and US associate partner, AU
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Binary microlensing event OGLE-2009-BLG-020 gives a verifiable mass, distance and orbit predictions

TL;DR: In this article, the first example of binary microlensing for which the parameter measurements can be verified (or contradicted) by future Doppler observations is presented, made possible by a confluence of two relatively unusual circumstances.
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Masses and Orbital Constraints for the OGLE-2006-BLG-109Lb,c Jupiter/Saturn Analog Planetary System

TL;DR: The OGLE-2006-BLG-109Lb,c was the first double planet system discovered with the gravitational microlensing method as discussed by the authors, which was the only multi-planet system discovered by any method with measured masses for the star and both planets.