The Nearby Supernova Factory project, based at Lawrence Berkeley National Laboratory, also has its Supernova Integrated Field Spectrograph (SNIFS) instrument mounted on UH88.
UH88 |
AU Microscopii harbors its own disk of dust, first resolved at optical wavelengths in 2003 by Paul Kalas and collaborators using the University of Hawaii 2.2-m telescope on Mauna Kea, Hawaii.