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Martin Dominik

Researcher at University of St Andrews

Publications -  414
Citations -  17326

Martin Dominik is an academic researcher from University of St Andrews. The author has contributed to research in topics: Gravitational microlensing & Planet. The author has an hindex of 62, co-authored 399 publications receiving 16221 citations. Previous affiliations of Martin Dominik include Max Planck Society & University of Groningen.

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First microlens mass measurement: PLANET photometry of EROS BLG-2000-5

TL;DR: In this paper, the authors analyzed PLANET photometric observations of the caustic-crossing binary-lens microlensing event, EROS BLG-2000-5, and found that modeling the observed light curve requires incorporation of the microlens parallax and the binary orbital motion.
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The extreme microlensing event OGLE-2007-BLG-224: terrestrial parallax observation of a thick-disk brown dwarf

Andrew Gould, +74 more
TL;DR: The OGLE-2007-BLG-224 microlensing event was observed in this article, from which the lens is a brown dwarf of mass M = 0.056 ± 0.004 M ☉, with a distance of 525 ± 40 pc and a transverse velocity of 113 ± 21 km s−1.
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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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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.