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About

M. Kubiak is a leading figure in astrophysical microlensing, with research centered on exoplanet detection, stellar binaries, and brown dwarfs. Their most-cited work, "OGLE-2008-BLG-510: first automated real-time detection of a weak microlensing anomaly" (2012, 25 citations), showcases a major contribution: pioneering the use of the Automated Robotic Terrestrial Exoplanet Microlensing Search (ARTEMiS) system to identify subtle, asymmetric light-curve anomalies in real time. This breakthrough enabled the rapid characterization of a microlensing event caused by either a brown dwarf or a stellar binary, demonstrating the power of automated pipelines for detecting low-mass objects. Kubiak’s work has significantly advanced the efficiency of microlensing surveys, reducing reliance on manual inspection and accelerating the discovery of exotic planetary and substellar systems. Their contributions have shaped how researchers approach real-time data analysis in the search for exoplanets, earning recognition for merging computational innovation with observational astronomy. With a citation impact that underscores the foundational nature of their methods, Kubiak remains a key contributor to the ongoing evolution of microlensing as a tool for probing the Milky Way’s hidden population of faint celestial bodies.