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About

Giancarlo Parodi is a leading figure in the development of next-generation X-ray optics, specializing in the fabrication and integration of lightweight, high-resolution mirror systems for space-based telescopes. His primary research focuses on the slumping of borosilicate glass sheets—a technique that enables the production of low-cost, lightweight mirrors crucial for future missions requiring unprecedented effective area and angular resolution. Parodi’s major contributions include pioneering the use of interfacing ribs for the accurate integration of segmented optics, a method that directly addresses the challenge of maintaining a 5 arc sec half-energy width (HEW) in large, long-focal-length telescopes. His 2013 paper on this topic, with 21 citations, is a foundational reference in the field. Earlier, his 2008 work on the XEUS (X-ray Evolving-Universe Spectroscopy Mission) design—cited 7 times—helped shape the mirror assembly concept for what would become ESA’s Athena mission, targeting collecting areas of 5–6 m² at 1 keV. Parodi’s research is instrumental in enabling the next leap in X-ray astronomy, balancing cost, weight, and performance to unlock deeper views of the hot, energetic universe.