Arid
DOI10.1117/12.788990
GLAS/NAOMI - ground-layer AO at the William Herschel Telescope
Benn, Chris1; Abrams, Don1; Agocs, Tibor1; Cano, Diego1; Gregory, Tom1; Guerra, Juan Carlos1; Martin, Olivier1; Morris, Tim2; Myers, Richard2; Rix, Samantha1; Rutten, Rene1; Skillen, Ian1; Skvarc, Jure1; Tulloch, Simon1
通讯作者Benn, Chris
会议名称Conference on Adaptive Optics Systems
会议日期JUN 23-28, 2008
会议地点Marseille, FRANCE
英文摘要

GLAS is an upgrade of the William Herschel Telescope's existing natural-guide-star (NGS) AO system NAOMI to incorporate a 20-W Rayleigh laser guide star (LGS) projected to an altitude of 1-5 kin. It is currently being commissioned on-sky, and we review here the current status of the project. GLAS/NAOMI delivers dramatic improvements in PSF in both the near-IR. (AO-corrected FWHM close to the diffraction limit, >similar to 0.15 arcsec) and in the optical (factor of similar to 2 reduction in FWHM). The performance is similar to that with NOS, and is consistent with predictions from modelling. The main advantage over NOS AO is the large gain in sky coverage (from similar to 1% to similar to 100% at galactic latitude 40 degrees). GLAS provides the first on-sky demonstration of closed-loop ground-layer AO (GLAO), and is the first Rayleigh LGS AO system to be offered for general use. at any telescope.


英文关键词Adaptive optics laser guide star Rayleigh GLAS NAOMI OASIS
来源出版物ADAPTIVE OPTICS SYSTEMS, PTS 1-3
ISSN0277-786X
EISSN1996-756X
出版年2008
卷号7015
ISBN978-0-8194-7225-0
出版者SPIE-INT SOC OPTICAL ENGINEERING
类型Proceedings Paper
语种英语
国家Spain;England
收录类别CPCI-S
WOS记录号WOS:000261491700054
WOS关键词ADAPTIVE OPTICS
WOS类目Astronomy & Astrophysics ; Computer Science, Interdisciplinary Applications ; Optics
WOS研究方向Astronomy & Astrophysics ; Computer Science ; Optics
资源类型会议论文
条目标识符http://119.78.100.177/qdio/handle/2XILL650/296955
作者单位1.Isaac Newton Grp, Apartado 321, Santa Cruz De La Palma 38700, Spain;
2.Univ Durham, Dept Phys, Sci Labs, Durham DH1 3LE, England
推荐引用方式
GB/T 7714
Benn, Chris,Abrams, Don,Agocs, Tibor,et al. GLAS/NAOMI - ground-layer AO at the William Herschel Telescope[C]:SPIE-INT SOC OPTICAL ENGINEERING,2008.
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