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About

Timothy Norton is an instrumental figure in observational astronomy, specializing in wide-field optical design and high-speed instrumentation for the detection of trans-Neptunian objects (TNOs). His career is defined by two major contributions: the commissioning of the MMT’s f/5 wide-field focus and the development of the TAOS II survey. Norton led the integration of the 6.5-meter MMT’s 1.7-meter secondary mirror and refractive corrector, achieving a 1° field of view for spectroscopy and delivering stellar images under 0.5 arcseconds FWHM—a feat that enabled transformative studies of the outer solar system. His most cited work (25 citations) details this system. Subsequently, Norton became the driving force behind TAOS II, a three-robotic-telescope project designed to monitor 10,000 stars simultaneously at 20 Hz, capturing stellar occultations by TNOs. His 2016 paper (12 citations) and 2014 paper (7 citations) outline the prototype and high-speed CMOS cameras, while his 2024 work reports on the final Mosaic camera performance. By engineering cameras capable of detecting rare occultation events, Norton has provided a statistically robust method to probe the distant Kuiper Belt, directly advancing our understanding of planetary formation.