Y. Nakada

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About

Y. Nakada is a key figure in astronomical instrumentation, best known for leading the development of the Kiso Wide Field Camera (KWFC), a facility instrument for the 105-cm Schmidt Telescope at the University of Tokyo’s Kiso Observatory. Their most-cited work, the 2012 paper detailing the KWFC’s design and capabilities, has garnered 39 citations and stands as a cornerstone of modern wide-field optical astronomy in Japan. By engineering a camera that exploits the Schmidt telescope’s large focal-plane area with an array of eight CCDs covering four square degrees, Nakada enabled transformative surveys of transient phenomena, variable stars, and near-Earth objects. This contribution has directly supported high-impact follow-up studies in time-domain astrophysics and cosmology. Beyond the KWFC, Nakada’s broader expertise in detector systems and telescope upgrades has made them an essential collaborator in Japanese observational astronomy. Their work exemplifies how innovative instrumentation can unlock new scientific frontiers, providing the astronomical community with a powerful tool for discovery and cementing Nakada’s legacy as a builder of the infrastructure that drives modern astrophysical research.