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About

Bart Willemse is a key figure in the development of next-generation astronomical instrumentation, specializing in the design and integration of complex multi-object spectrographs. His primary research focus is on the mechanical and optical systems that enable large-scale spectroscopic surveys, with his most notable work centered on the MOONS (Multi-Object Optical and Near-infrared Spectrograph) instrument for the ESO Very Large Telescope. Willemse’s major contributions include leading the build and integration of the MOONS Fibre Positioning Module (FPM), a sophisticated system that precisely configures 1000 optical fibres using individual robotic positioners. This technology is critical for achieving the high multiplexing capability that allows MOONS to simultaneously observe nearly a thousand celestial objects. His work on the FPM (7 citations) and the overall instrument integration (4 citations) has been instrumental in advancing the VLT’s observational power. By engineering the robotic positioning system, Willemse has helped enable transformative studies in galactic archaeology, galaxy evolution, and cosmology, cementing his role as a vital contributor to one of the most ambitious multi-object spectrographs ever built.