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Title: Performance of the Keck Observatory adaptive optics system

Journal Article · · Applied Optics

In this paper, the adaptive optics (AO) system at the W.M. Keck Observatory is characterized. The authors calculate the error budget of the Keck AO system operating in natural guide star mode with a near infrared imaging camera. By modeling the control loops and recording residual centroids, the measurement noise and band-width errors are obtained. The error budget is consistent with the images obtained. Results of sky performance tests are presented: the AO system is shown to deliver images with average Strehl ratios of up to 0.37 at 1.58 {micro}m using a bright guide star and 0.19 for a magnitude 12 star.

Research Organization:
Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Sponsoring Organization:
USDOE
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
859914
Report Number(s):
UCRL-JRNL-201902; APOPAI; TRN: US200523%%109
Journal Information:
Applied Optics, Vol. 43, Issue 29; ISSN 0003-6935
Country of Publication:
United States
Language:
English

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