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About

M. Bagaglia is an instrumental figure in the advancement of infrared astronomy, with a career focused on developing cutting-edge observational facilities for extreme environments. His primary research areas include the design and construction of ground-based infrared telescopes and high-speed optical instrumentation for transient astrophysical phenomena. Bagaglia’s most significant contribution is his leadership in the International Robotic Antarctic Infrared Telescope (IRAIT) project, which demonstrated that Dome C on the Antarctic plateau offers the best terrestrial conditions for thermal and far-infrared observations (2.3–300 μm) due to its exceptional coldness, low sky brightness, and minimal water vapor. This work, cited 25 times, laid the groundwork for future Antarctic observatories. He also made a major impact with the REM optical slitless spectrograph (ROSS), a fast-response instrument on the Rapid Eye Mount telescope in Chile, enabling simultaneous optical-near-infrared observations of gamma-ray bursts (GRBs). With 23 citations, this system proved critical for understanding the physics of these high-energy events. Bagaglia’s achievements highlight his role in pushing the boundaries of observational astronomy, creating tools that allow researchers to probe the universe from the most challenging and rewarding sites on Earth.