Paper
31 May 1994 Performance and results of the COME-ON+ adaptive optics system at the ESO 3.6-m telescope
Gerard Rousset, Jean-Luc Beuzit, Norbert N. Hubin, Eric Gendron, Pierre-Yves Madec, Corinne Boyer, Jean-Paul Gaffard, Jean-Claude Richard, M. Vittot, Pierre Gigan, Pierre J. Lena
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, Jean-Luc Beuzit, Norbert N. Hubin, Eric Gendron, Pierre-Yves Madec, Corinne Boyer, Jean-Paul Gaffard, Jean-Claude Richard, M. Vittot, Pierre Gigan, and 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); https://doi.org/10.1117/12.176020
Lens.org Logo
CITATIONS
Cited by 11 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Stars

Cameras

Adaptive optics

Mirrors

Wavefronts

Astronomy

Wavefront sensors

RELATED CONTENT

CRAO: a compact and refractive adaptive-optics
Proceedings of SPIE (August 04 2014)
MCAO with LINC NIRVANA at LBT preparing for first...
Proceedings of SPIE (September 02 2016)
Status of the NGS adaptive optic system at the MMT...
Proceedings of SPIE (October 25 2004)
Adaptive optics for the CHARA array
Proceedings of SPIE (September 13 2012)
Using CODE V to model adaptive optics
Proceedings of SPIE (October 22 2004)

Back to Top