Performance of the Keck Observatory adaptive optics system
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
Similar Records
Characterization of Adaptive Optics at Keck Observatory
eXtreme Adaptive Optics Planet Imager: Overview and status
Issues in the design and optimization of adaptive optics and laser guide stars for the Keck Telescopes
Conference
·
Thu Jul 24 00:00:00 EDT 2003
·
OSTI ID:859914
eXtreme Adaptive Optics Planet Imager: Overview and status
Conference
·
Wed Aug 18 00:00:00 EDT 2004
·
OSTI ID:859914
+19 more
Issues in the design and optimization of adaptive optics and laser guide stars for the Keck Telescopes
Conference
·
Tue Mar 01 00:00:00 EST 1994
·
OSTI ID:859914