The DEIMOS spectrograph for the Keck II Telescope: integration and testing

Autor: Vernon Wallace, David Kirk Gilmore, Jack Osborne, Gregory D. Wirth, Ricardo P. Schiavon, Jeffrey P. Lewis, Sandra M. Faber, Barry Alcott, Mingzhi Wei, Alison L. Coil, William Deich, Andrew C. Phillips, Robert I. Kibrick, Marc Davis, Richard J. Stover, Christopher A.F. Wright, David Cowley, Jeffrey A. Newman, Dean Tucker, T. Cantrall, Ken Dietsch, De A. Clarke, Jim Burrous, Carol Ann Harper, Molly McVeigh, David F. Hilyard, Steven L. Allen
Přispěvatelé: Iye, Masanori, Moorwood, Alan FM
Rok vydání: 2003
Předmět:
Zdroj: Proceedings of SPIE, vol 4841, iss 3
Proceedings of SPIE-The International Society for Optical Engineering, vol 4841, iss 3
Faber, Sandra M; Phillips, Andrew C; Kibrick, Robert I; Alcott, Barry; Allen, Steven L; Burrous, Jim; et al.(2003). The DEIMOS spectrograph for the Keck II Telescope: integration and testing. Instrument Design and Performance for Optical/Infrared Ground-based Telescopes, 4841(3), 1657-1669. doi: 10.1117/12.460346. UC Santa Cruz: Retrieved from: http://www.escholarship.org/uc/item/84m7z4h6
Popis: The DEIMOS spectrograph is a multi-object spectrograph being built for Keck II. DEIMOS was delivered in February 2002, became operational in May, and is now about three-quarters of the way through its commissioning period. This paper describes the major problems encountered in completing the spectrograph, with particular emphasis on optical quality and image motion. The strategies developed to deal with these problems are described. Overall, commissioning is going well, and it appears that DEIMOS will meet all of its major performance goals.
Databáze: OpenAIRE