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Proceedings Paper

Performance of the W.M. Keck Observatory Natural Guide Star Adaptive Optic Facility: the first year at the telescope
Author(s): Peter L. Wizinowich; D. Scott Acton; Olivier Lai; John Gathright; William Lupton; Paul J. Stomski Jr.
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Paper Abstract

First light for the Keck II Natural Guide Star (NGS) Adaptive Optics (AO) facility was on the night of February 4, 1999. On the firs attempt at closing the AO loops the image full-width- at-half-maximum (FWHM) went from 0.6 to 0.04 arcsec at H-band (1.65 micrometer wavelength), with a Strehl ratio of 25%. The AO system became an officially scheduled Keck science facility in August 1999; 30 science nights are scheduled in the first half of 2000. The primary purpose of this paper is to present results from this first year at the telescope.

Paper Details

Date Published: 7 July 2000
PDF: 12 pages
Proc. SPIE 4007, Adaptive Optical Systems Technology, (7 July 2000); doi: 10.1117/12.390368
Show Author Affiliations
Peter L. Wizinowich, W.M. Keck Observatory (United States)
D. Scott Acton, W.M. Keck Observatory (United States)
Olivier Lai, Canada-France-Hawaii Telescope Corp. (United States)
John Gathright, W.M. Keck Observatory (United States)
William Lupton, W.M. Keck Observatory (United States)
Paul J. Stomski Jr., W.M. Keck Observatory (United States)

Published in SPIE Proceedings Vol. 4007:
Adaptive Optical Systems Technology
Peter L. Wizinowich, Editor(s)

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