31 May 1994 Performance and results of the COME-ON+ adaptive optics system at the ESO 3.6-m telescope
Author Affiliations +
Abstract
The COME-ON+ adaptive optics system was set up on the ESO 3.6-meter telescope for two technical runs (in December 1992 and April 1993) and is now routinely used for astronomical observations. This system is an upgrade of the COME-ON adaptive optics prototype system. During the technical runs, images were recorded in the V, I, J, K and L' spectral bands. Currently, the best resolution obtained is 0.1' in H (1.65 micrometers ) under bad seeing conditions (seeing > 1' and averaged wind speed > 10 m/s) and reference star magnitudes of 6 to 8. The corresponding Strehl ratio is 35%. 70% Strehl ratio was obtained at 2.2 micrometers (K band). At 0.9 micrometers (I band), in the partial correction regime, the resolution is of the order of 0.2' for 0.8' seeing and 10 m/s averaged wind speed. The optimized modal control has been used on faint reference stars. The limiting magnitude (in V band) for wavefront sensing has been measured to 14 and 15 depending on the spectral type of the reference star and the seeing conditions for a low frequency tip-tilt correction.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gerard Rousset, Gerard Rousset, Jean-Luc Beuzit, Jean-Luc Beuzit, Norbert N. Hubin, Norbert N. Hubin, Eric Gendron, Eric Gendron, Pierre-Yves Madec, Pierre-Yves Madec, Corinne Boyer, Corinne Boyer, Jean-Paul Gaffard, Jean-Paul Gaffard, Jean-Claude Richard, Jean-Claude Richard, M. Vittot, M. Vittot, Pierre Gigan, Pierre Gigan, Pierre J. Lena, Pierre J. Lena, } "Performance and results of the COME-ON+ adaptive optics system at the ESO 3.6-m telescope", Proc. SPIE 2201, Adaptive Optics in Astronomy, (31 May 1994); doi: 10.1117/12.176020; https://doi.org/10.1117/12.176020
PROCEEDINGS
11 PAGES


SHARE
RELATED CONTENT

MCAO with LINC NIRVANA at LBT preparing for first...
Proceedings of SPIE (September 01 2016)
Adaptive optics for the CHARA array
Proceedings of SPIE (September 12 2012)
Using CODE V to model adaptive optics
Proceedings of SPIE (October 21 2004)
W.M. Keck Observatory adaptive optics program
Proceedings of SPIE (May 30 1994)
Adaptive optics for the Gran Telescopio Canarias
Proceedings of SPIE (September 10 1998)

Back to Top