AOLI: Adaptive Optics plus Lucky Imager for the WHT (4.2m) and GTC (10.5m) Telescopes.
AOLI: Adaptive Optics plus Lucky Imager for the WHT (4.2m) and GTC (10.5m) Telescopes.
批准号:
ST/K002368/1
负责人:
Craig Mackay
金额:
$17.82万
依托单位:
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2012
资助国家:
英国
项目状态:
已结题
起止时间:
2012 至 --
中文摘要
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英文摘要
The highest resolution images of faint targets ever taken in the visible or near infrared were obtained by combining Lucky Imaging with low order adaptive optics. This proposal is to develop further the technologies needed for an innovative approach to wavefront sensing that will allow dramatically fainter reference stars to be used than with conventional Shack-Hartmann sensors. These will be incorporated in an instrument to be used initially on the WHT 4.2 m with the potential to move to the GTC 10 meter telescope on La Palma. Using only faint natural guide stars, angular resolution as good as 15 milliarcseconds in the GTC and 40 milliarcseconds on the WHT in I-band will be obtained over a substantial fraction of the northern sky. The instrument is part of a collaboration led by the Institute of Astronomy of the University of Cambridge, with the IAC (La Laguna), UPCT (Cartagena), University of Cologne and the staff of the ING (La Palma). This project is central to the aims and aspirations of the STFC science program for astronomy. It also supports the strongly expressed wish to integrate activities of the ING with those of the IAC/GranteCan telescope on La Palma. The project builds on several exciting new technologies that have made great strides over the last year in Cambridge. In particular, much higher selection percentages are now achieved without loss of resolution. The instrument proposed here will start as a visitor instrument permanently resident on the island, with the medium-term goal of transitioning to a common user facility for use on the two La Palma telescopes. The instrument first light on the WHT will be ~18 months after kick-off and fully operational by the end of 3 years. The costs will be shared between the UK and collaborators in Spain and Germany. This proposal is for a total of £138K from STFC (£167K FEC) including components, travel and salaries. The entire project is expected to cost in the region of £1.5 million.
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DOI:
10.1093/mnras/stt507
发表时间:
2013-03
期刊:
Monthly Notices of the Royal Astronomical Society
影响因子:
4.8
作者:
[C. Mackay]
通讯作者:
C. Mackay
Wavefront phase retrieval with non-linear curvature sensors
使用非线性曲率传感器进行波前相位检索
DOI:
10.1093/mnras/sts472
发表时间:
2013
期刊:
Monthly Notices of the Royal Astronomical Society
影响因子:
4.8
作者:
[Aisher P]
通讯作者:
Aisher P
Laboratory and telescope demonstration of the TP3-WFS for the adaptive optics segment of AOLI
用于 AOLI 自适应光学部分的 TP3-WFS 的实验室和望远镜演示
DOI:
10.1093/mnras/stx262
发表时间:
2017
期刊:
Monthly Notices of the Royal Astronomical Society
影响因子:
4.8
作者:
[Colodro-Conde C]
通讯作者:
Colodro-Conde C
DOI:
10.1093/mnras/stt885
发表时间:
2013-05
期刊:
Monthly Notices of the Royal Astronomical Society
影响因子:
4.8
作者:
[F. Faedi;Tim D. Staley;Y. G. M. Chew;D. Pollacco;S. Dhital;S. Dhital;S. Barros;I. Skillen;L. Hebb;Craig D. Mackay;Christopher A. Watson]
通讯作者:
F. Faedi;Tim D. Staley;Y. G. M. Chew;D. Pollacco;S. Dhital;S. Dhital;S. Barros;I. Skillen;L. Hebb;Craig D. Mackay;Christopher A. Watson
The Adaptive Optics Lucky Imager: Diffraction limited imaging at visible wavelengths with large ground-based telescopes
自适应光学幸运成像仪:使用大型地面望远镜在可见波长下进行衍射限制成像
DOI:
--
发表时间:
2015
期刊:
American Astronomical Society Meeting Abstracts #225
影响因子:
--
作者:
[Crass Jonathan]
通讯作者:
Crass Jonathan
共 8 条
Ground-Based High Resolution Imaging in the Visible: The Cambridge Lucky Aperture Synthesis Instrument
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批准号:ST/F00379X/1
-
项目类别:Research Grant
-
资助金额:$65.21万
-
财政年份:2008
-
负责人:Craig Mackay
-
依托单位:
海外基金