NAOMI: a low-order adaptive optics system for the VLT Interferometer

被引:4
作者
Gonte, Frederic Yves J. [1 ]
Alonso, Jaime [1 ]
Aller-Carpentier, Emmanuel [1 ]
Andolfato, Luigi [1 ]
Berger, Jean-Philippe [1 ]
Cortes, Angela [1 ]
Delplancke-Strobele, Francoise [1 ]
Donaldson, Rob [1 ]
Dorn, Reinhold J. [1 ]
Dupuy, Christophe [1 ]
Egner, Sebastian E. [1 ]
Huber, Stefan [1 ]
Hubin, Norbert [1 ]
Kirchbauer, Jean-Paul [1 ]
Le Louarn, Miska [1 ]
Lilley, Paul [1 ]
Jolley, Paul [1 ]
Martis, Alessandro [1 ]
Paufique, Jerome [1 ]
Pasquini, Luca [1 ]
Quentin, Jutta [1 ]
Ridings, Robert [1 ]
Reyes, Javier [1 ]
Shchkaturov, Pavel [1 ]
Suarez, Marcos [1 ]
Thanh Phan Duc [1 ]
Valdes, Guillermo [1 ]
Woillez, Julien [1 ]
Le Bouquin, Jean-Baptiste [2 ]
Beuzit, Jean-Luc [2 ]
Rochat, Sylvain [2 ]
Verinaud, Christophe [2 ]
Moulin, Thibaut [2 ]
Delboulbe, Alain [2 ]
Michaud, Laurence [2 ]
Correia, Jean-Jacques [2 ]
Roux, Alain [2 ]
Maurel, Didier [2 ]
Stadler, Eric [2 ]
Magnard, Yves [2 ]
机构
[1] European Southern Observ, Garching, Germany
[2] Inst Planetol & Astrophys Grenoble, Grenoble, France
来源
OPTICAL AND INFRARED INTERFEROMETRY AND IMAGING V | 2016年 / 9907卷
关键词
Adaptive Optics; Interferometry; Auxiliary Telescopes;
D O I
10.1117/12.2233993
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The New Adaptive Optics Module for Interferometry (NAOMI) will be developed for and installed at the 1.8-metre Auxiliary Telescopes (ATs) at ESO Paranal. The goal of the project is to equip all four ATs with a low-order Shack-Hartmann adaptive optics system operating in the visible. By improving the wavefront quality delivered by the ATs for guide stars brighter than R = 13 mag, NAOMI will make the existing interferometer performance less dependent on the seeing conditions. Fed with higher and more stable Strehl, the fringe tracker(s) will achieve the fringe stability necessary to reach the full performance of the second-generation instruments GRAVITY and MATISSE.
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页数:12
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