Bibcode
Talbot, Gordon; Abrams, Don Carlos; Apostolakos, Nikolaos; Bassom, Richard; Blackburn, Colin; Blanken, Maarten; Cano Infantes, Diego; Chopping, Alan; Dee, Kevin; Dipper, Nigel; Elswijk, Eddy; Enthoven, Bernard; Gregory, Thomas; ter Horst, Rik; Humphreys, Ron; Idserda, Jan; Jolley, Paul; Kuindersma, Sjouke; McDermid, Richard; Morris, Tim; Myers, Richard; Pico, Sergio; Pragt, Johan; Rees, Simon; Rey, Jürg; Reyes, Marcos; Rutten, René; Schoenmaker, Ton; Skvarc, Jure; Tromp, Niels; Tulloch, Simon; Veninga, Auke
Bibliographical reference
Advances in Adaptive Optics II. Edited by Ellerbroek, Brent L.; Bonaccini Calia, Domenico. Proceedings of the SPIE, Volume 6272, pp. 62722H (2006).
Advertised on:
7
2006
Citations
0
Refereed citations
0
Description
The GLAS (Ground-layer Laser Adaptive-optics System) project is to
construct a common-user Rayleigh laser beacon that will work in
conjunction with the existing NAOMI adaptive optics system, instruments
(near IR imager INGRID, optical integral field spectrograph OASIS,
coronagraph OSCA) and infrastructure at the 4.2-m William Herschel
Telescope (WHT) on La Palma. The laser guide star system will increase
sky coverage available to high-order adaptive optics from ~1% to
approaching 100% and will be optimized for scientific exploitation of
the OASIS integral-field spectrograph at optical wavelengths.
Additionally GLAS will be used in on-sky experiments for the application
of laser beacons to ELTs. This paper describes the full range of
engineering of the project ranging through the laser launch system,
wavefront sensors, computer control, mechanisms, diagnostics, CCD
detectors and the safety system. GLAS is a fully funded project, with
final design completed and all equipment ordered, including the laser.
Integration has started on the WHT and first light is expected summer
2006.