Conceptual design and performance of the multi-conjugate adaptive optics module for the European Extremely Large Telescope

被引:11
|
作者
Diolaiti, Emiliano [1 ]
Conan, Jean-Marc [2 ]
Foppiani, Italo [1 ,3 ]
Marchetti, Enrico [4 ]
Baruffolo, Andrea [5 ]
Bellazzini, Michele [1 ]
Bregoli, Giovanni [1 ]
Butler, Christopher R. [6 ]
Ciliegi, Paolo [1 ]
Cosentino, Giuseppe [3 ]
Delabre, Bernard [4 ]
Lombini, Matteo [1 ,3 ]
Petit, Cyril [2 ]
Robert, Clelia [2 ]
Rossettini, Pierfrancesco [7 ]
Schreiber, Laura [3 ]
Tomelleri, Raffaele [7 ]
Biliotti, Valdemaro [8 ]
D'Odorico, Sandro [4 ]
Fusco, Thierry [2 ]
Hubin, Norbert [4 ]
Meimon, Serge [2 ]
机构
[1] INAF Osservatorio Astron Bologna, Via Ranzani 1, I-40127 Bologna, Italy
[2] Off Natl Etud & Rech Aerosp, F-92322 Chatillon, France
[3] Univ Bologna, Dipartmento Astron, I-40127 Bologna, Italy
[4] European Org Astron Res Southern Hemisphere, D-85748 Munich, Germany
[5] Osserv Astron Padova, INAF, I-35122 Padua, Italy
[6] Inst Astrofis Spaziale & Fis Cosm, INAF, I-40129 Bologna, Italy
[7] Tomelleri Srl, I-37069 Verona, Italy
[8] Osserv Astrofis Arcetri, INAF, I-50125 Florence, Italy
来源
ADAPTIVE OPTICS SYSTEMS II | 2010年 / 7736卷
关键词
Extremely Large Telescopes; E-ELT; multi-conjugate adaptive optics; laser guide stars; sky coverage;
D O I
10.1117/12.857634
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The Multi-conjugate Adaptive Optics RelaY (MAORY) for the European Extremely Large Telescope (E-ELT) provides a corrected field of view of up to 2 arcmin diameter over the wavelength range 0.8-2.4 mu m. It is expected to achieve a correction of high quality and uniformity with high sky coverage: with a seeing of 0.8 arcsec in the visible, the expected Strehl Ratio averaged over a 1 arcmin field is approximately 50% at 2.16 mu m wavelength over 50% of the sky at the Galactic Pole. Wavefront correction is obtained by means of the E-ELT adaptive mirrors M4/M5 and of two post-focal deformable mirrors conjugated at 4km and 12.7km from the telescope pupil. Wavefront sensing is performed by 6 Sodium laser guide stars and by 3 natural guide stars, used to measure atmospheric and windshake tilt and to provide a reference for the focus and for the low-order aberrations induced by the Sodium layer. MAORY is located on the E-ELT Nasmyth platform and has a gravity invariant port, feeding the high angular resolution camera MICADO, and a lateral port for a detached instrument as the infrared spectrograph SIMPLE.
引用
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页数:9
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