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About

Y. Muraki is a leading figure in gravitational microlensing, with a career dedicated to detecting and characterizing elusive astronomical objects such as brown dwarfs and stellar binaries. His primary research focuses on the real-time analysis of microlensing anomalies, which are subtle deviations in stellar brightness caused by the gravitational field of an intervening object. Muraki’s most significant contribution is the development and application of automated detection systems, most notably through the ARTEMiS (Automated Robotic Terrestrial Exoplanet Microlensing Search) project. His pioneering work on the event OGLE-2008-BLG-510 (25 citations) marked the first automated real-time detection of a weak microlensing anomaly, demonstrating the power of robotic telescopes to identify complex signals like those from a brown dwarf or binary system. This breakthrough has enabled faster, more efficient follow-up observations. Further cementing his impact, Muraki led the analysis of OGLE-2015-BLG-0060 (5 citations), a stellar binary event observed by 13 telescopes worldwide. His work has been instrumental in advancing our understanding of low-mass objects and binary star systems, showcasing the synergy between automated detection and multi-telescope collaboration.