7 August 2014 CHARA array adaptive optics II: non-common-path correction and downstream optics
Author Affiliations +
We describe a back-end Adaptive Optics system for the CHARA Array called Lab-AO intended to compensate for non-common path errors between the AO system at the telescopes and the final beam combining area some hundreds of meters away. The system is an on-axis, very small field of view, low order system that will work on star light if enough is present, or will make use of a blue light beacon sent from the telescope towards the laboratory if not enough star light is available. The first of six of these system has been installed and has recently been tested on the sky. Another five will be built for the remaining telescopes later this year.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Theo ten Brummelaar, Theo ten Brummelaar, Xiao Che, Xiao Che, Harold McAlister, Harold McAlister, Michael Ireland, Michael Ireland, John Monnier, John Monnier, Denis Mourard, Denis Mourard, Stephen Ridgway, Stephen Ridgway, Judit Sturmann, Judit Sturmann, Laszlo Sturmann, Laszlo Sturmann, Nils Turner, Nils Turner, Peter Tuthill, Peter Tuthill, } "CHARA array adaptive optics II: non-common-path correction and downstream optics", Proc. SPIE 9148, Adaptive Optics Systems IV, 91484Q (7 August 2014); doi: 10.1117/12.2056662; https://doi.org/10.1117/12.2056662


Low-cost adaptive optics for astronomical applications
Proceedings of SPIE (September 24 2001)
Ground-layer adaptive optics performance in Antarctica
Proceedings of SPIE (October 24 2004)
Performance and test results of a 61 element adaptive optics...
Proceedings of SPIE (September 04 2002)
Predictors in the servo-loop of an AO system
Proceedings of SPIE (September 10 1998)

Back to Top