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About

Sebastiaan Fransen is a key figure in the development of next-generation X-ray optics for space-based astrophysics. His research centers on the design, technology preparation, and system-level implementation of advanced telescope mirrors, particularly for high-energy missions. Fransen’s major contributions lie in advancing Silicon Pore Optics (SPO) technology, a novel approach that enables lightweight, high-resolution X-ray mirrors for future observatories. He has been instrumental in the mission studies for the Advanced Telescope for High ENergy Astrophysics (ATHENA), a cornerstone of ESA’s Cosmic Vision programme. His work on the ATHENA optics, including the 2015 paper outlining the system architecture, has shaped the mission’s technical roadmap. With his most-cited paper from 2019 accumulating 8 citations, Fransen’s research directly supports the realization of ATHENA, which promises to revolutionize our understanding of hot, energetic processes in the Universe. His efforts bridge cutting-edge optical engineering and space science, making him a vital contributor to Europe’s next large-class X-ray observatory.