Laboratory and telescope demonstration of the TP3-WFS for the adaptive optics segment of AOLI
Laboratory and telescope demonstration of the TP3-WFS for the adaptive optics segment of AOLI
复制标题
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
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发表时间:
2017
影响因子:
4.8
通讯作者:
Colodro-Conde C
中科院分区:
文献类型:
--
作者:
Colodro-Conde C
Adaptive Optics Lucky Imager (AOLI) is a state-of-the-art instrument that combines adaptive optics (AO) and lucky imaging (LI) with the objective of obtaining diffraction-limited images in visible wavelength at mid- and big-size ground-based telescopes. The key innovation of AOLI is the development and use of the new Two Pupil Plane Positions Wavefront Sensor (TP3-WFS). The TP3-WFS, working in visible band, represents an advance over classical wavefront sensors such as the Shack-Hartmann WFS because it can theoretically use fainter natural reference stars, which would ultimately provide better sky coverages to AO instruments using this newer sensor. This paper describes the software, algorithms and procedures that enabled AOLI to become the first astronomical instrument performing real-time AO corrections in a telescope with this new type of WFS, including the first control-related results at the William Herschel Telescope.
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影响因子:
0.9
作者:
T. Berkefeld;D. Schmidt;D. Soltau;O. Lühe;F. Heidecke
通讯作者:
T. Berkefeld;D. Schmidt;D. Soltau;O. Lühe;F. Heidecke
DOI:
10.1016/s0031-8914(34)80259-5
发表时间:
1934-05
期刊:
Physica D: Nonlinear Phenomena
影响因子:
--
作者:
von F. Zernike
通讯作者:
von F. Zernike
DOI:
--
发表时间:
2010
期刊:
Astronomical Telescopes + Instrumentation
影响因子:
--
作者:
O. Guyon;F. Martinache;V. Garrel;F. Vogt;K. Yokochi;Takashi Yoshikawa
通讯作者:
Takashi Yoshikawa
DOI:
--
发表时间:
2013
期刊:
影响因子:
--
作者:
J. J. Fernández;Alberto Lastra Sedano;S. Chueca;Javier Sanz Gil;J. Rodríguez
通讯作者:
J. Rodríguez
影响因子:
1.9
作者:
M. V. van Dam;R. Lane
通讯作者:
R. Lane