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The Hawaii K-band Galaxy Survey from the 1990s was a near-infrared astronomical survey of select survey fields using IRCAM on United Kingdom Infrared Telescope (UKIRT) and NICMOS3 on the UH88 telescope, with photometry including the K band and optical bands and follow-up spectrography using 2dF on the Anglo-Australian Telescope (AAT). Distant galaxies were discovered, inducing further study.