Final two-stage MOAO on-sky demonstration with CANARY

被引:7
|
作者
Gendron, E. [1 ]
Morris, T. [2 ]
Basden, A. [2 ]
Vidal, F. [1 ]
Atkinson, D. [7 ]
Bitene, U. [2 ]
Buey, T. [1 ]
Chemla, F.
Cohen, M. [3 ]
Dickson, C. [7 ]
Dipper, N. [2 ]
Feautrier, P. [4 ,6 ]
Gach, J-L [4 ,5 ]
Gratadour, D. [1 ]
Henry, D. [7 ]
Huet, J-M [3 ]
Morel, C. [1 ]
Morris, S. [2 ]
Myers, R. [2 ]
Osborn, J. [2 ]
Perret, D. [1 ]
Reeves, A. [2 ]
Rousset, G. [1 ]
Sevin, A. [1 ]
Stadler, E. [4 ,6 ]
Talbot, G. [2 ]
Todd, S. [7 ]
Younger, E. [2 ]
机构
[1] UPMC, Univ Paris Diderot, CNRS, LESIA,Obs Paris, 5 P Janssen, F-92190 Meudon, France
[2] Univ Durham, Ctr Adv Instrumentat, South Rd, Durham DH1 3LE, England
[3] UPMC, Univ Paris Diderot, CNRS, GEPI,Obs Paris, 5 P Janssen, F-92190 Meudon, France
[4] First Light Imaging SAS, 100 Impasse Houilleres, F-13590 Meyreuil, France
[5] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France
[6] Inst Planetol & Astrophys Grenoble, UMR 5274, BP 53, F-38041 Grenoble 9, France
[7] Royal Observ, UKATC, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland
来源
ADAPTIVE OPTICS SYSTEMS V | 2016年 / 9909卷
关键词
tomography; ELT; instrumentation; laser guide star; adaptive optics; wave-front sensing; WAVE-FRONT SENSOR; DEFORMABLE MIRROR; LASER;
D O I
10.1117/12.2231432
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
CANARY is an on-sky Laser Guide Star (LGS) tomographic AO demonstrator in operation at the 4.2m William Herschel Telescope (WHT) in La Palma. From the early demonstration of open-loop tomography on a single deformable mirror using natural guide stars in 2010, CANARY has been progressively upgraded each year to reach its final goal in July 2015. It is now a two-stage system that mimics the future E-ELT: a GLAO-driven woofer based on 4 laser guide stars delivers a ground-layer compensated field to a figure sensor locked tweeter DM, that achieves the final on-axis tomographic compensation. We present the overall system, the control strategy and an overview of its on-sky performance.
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页数:17
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