Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

Results of the COME-ON experiment

Not Accessible

Your library or personal account may give you access

Abstract

The last results obtained with the adaptive optics (AO) system COME-ON are reported here. A new set-up, pushing the servo-loop bandwidth up to 25 Hz, allowed to get diffraction limited long exposure images down to 1.7 μm on a 3.6-m telescope (i.e. 96 milliarcsec). Compared with the turbulent case, gains in Strehl ratio (S) up to 13 are reported. Profile of partially corrected images are shown, which confirm partly the predicted profiles. These results are based on data collected at the ESO 3.6-m telescope, La Silla, Chile, on April 1991.

© 1992 Optical Society of America

PDF Article
More Like This
The Come-On-Plus Project

G. Rousset, P-Y. Madec, J-L. Beuzit, J-G. Cuby, P. Gigan, P. Lena, F. Rigaut, C. Boyer, J-P. Gaffard, J-C. Richard, M. Vittot, E. Gendron, N. Hubin, and F. Merkle
AWA1 Adaptive Optics for Large Telescopes (AOLT) 1992

Compensated imaging using hybrid techniques: experiment and results

Marsha F. Bilmont, Mark A. Von Bokern, David G. Voelz, Michael C. Roggemann, and John P. Albetski
AWA3 Adaptive Optics for Large Telescopes (AOLT) 1992

Atmospheric wavefront measurements and evaluation of adaptive optics efficiency

P.Y. Madec, G. Rousset, and M. Séchaud
AThA5 Adaptive Optics for Large Telescopes (AOLT) 1992

Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.