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About

M. V. Pruzhinskaya is a leading astrophysicist specializing in robotic optical astronomy, gamma-ray bursts (GRBs), and transient phenomena. Her major contributions center on the development and scientific exploitation of the MASTER-II network of robotic telescopes, which she helped create to enable rapid, autonomous follow-up of cosmic explosions. Her 2013 paper describing the MASTER-II network (63 citations) established the system’s capability for studying prompt optical emission from GRBs and conducting wide-field sky surveys. In a landmark 2015 study (38 citations), she demonstrated the network’s unique ability to automatically react to poorly localized Fermi GBM alerts, achieving early optical afterglow discovery within a 137 square-degree error box—a feat no other observatory could match. Pruzhinskaya also pioneered optical polarization observations with MASTER (22 citations), adding a new dimension to transient characterization. Her work has significantly advanced real-time astrophysics, enabling rapid identification of GRB counterparts and opening new windows into the physics of relativistic jets. Through these achievements, she has established herself as a key figure in the emerging field of robotic telescope networks and time-domain astronomy.