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About

S. Castellini is a pioneering figure in Antarctic astronomy, whose work has been instrumental in establishing Dome C as a premier site for infrared observation. His key research areas encompass the development and robotization of telescopes for extreme environments, specifically focusing on thermal and far-infrared astronomy. Castellini’s major contribution is his leadership in the International Robotic Antarctic Infrared Telescope (IRAIT) project, which demonstrated that Dome C’s exceptional coldness, low sky brightness, and minimal water vapor make it the best Earth-based location for observations in the 2.3–300 μm range. His 2006 paper on IRAIT, with 25 citations, remains a foundational reference for site characterization. Further impact is shown in his 2007 work on telescope robotization (16 citations), which synthesized the challenges and solutions for operating instruments at Concordia Station. By addressing the unique hurdles of remote, automated night-time operations in the harsh Antarctic climate, Castellini has paved the way for a new generation of robotic observatories, enabling continuous, high-quality infrared astronomy from the most inhospitable yet scientifically rewarding locations on Earth.