Comptes Rendus
MCAO for very large telescopes/OAMC pour les très grands télescopes
MAD: practical implementation of MCAO concepts
[MAD : implementation pratique de concepts en OAMC]
Comptes Rendus. Physique, Volume 6 (2005) no. 10, pp. 1118-1128.

L'ESO ainsi que des instituts de recherche externes ont développé MAD (le Démonstrateur d'Optique Adaptative Multi-Conjuguée) pour effectuer la correction d'optique adaptative grand champ (2′ en bande K). Le but de MAD est de démontrer sur le ciel la faisabilité de la technique d'OAMC et d'évaluer ses points critiques pour l'instrumentation de 2eme génération pour le VLT et pour le télescope OWL. MAD sera installé au VLT pour effectuer des observations sur le ciel. MAD utilise deux miroirs deformables et deux senseurs de front d'onde multi-référence avec des étoiles-guide naturelles. Dans cet article nous présentons la conception du démonstrateur, quelques aspects de l'étalonnage de MAD et les premiers résultats en boucle fermée dans les configurations mono-conjugée (SCAO) et correction de la couche au sol (GLAO).

The European Southern Observatory (ESO) together with external research institutes have built a Multi-Conjugate Adaptive Optics (MCAO) Demonstrator (MAD) to perform wide field-of-view adaptive optics correction (2′ in K band). The aim of MAD is to demonstrate the on-sky feasibility of the MCAO technique and to evaluate its critical aspects in the framework of both the 2nd generation instrumentation for the Very Large Telescope (VLT) and the Overwhelmingly Large Telescope (OWL). The MAD module will be installed on the VLT to perform on-sky observations. MAD comprises two deformable mirrors and two different multi-reference wavefront sensors with natural guide stars. In this article we present the MAD design, some aspects of the MAD calibration and the first closed-loop results in the laboratory in Single Conjugated Adaptive Optics (SCAO) and Ground Layer Adaptive Optics (GLAO) configurations.

Publié le :
DOI : 10.1016/j.crhy.2005.11.002
Keywords: Multi-Conjugate Adaptive Optics, Wavefront sensors, Layer oriented, Ground Layer Adaptive Optics
Mot clés : Optique Adaptative Multi-Conjugée, Senseurs de Front d'Onde
Enrico Marchetti 1 ; Roland Brast 1 ; Bernard Delabre 1 ; Rob Donaldson 1 ; Enrico Fedrigo 1 ; Christoph Frank 1 ; Norbert Hubin 1 ; Johann Kolb 1 ; Miska Le Louarn 1 ; Jean-Louis Lizon 1 ; Sylvain Oberti 1 ; Fernando Quirós-Pacheco 1 ; Roland Reiss 1 ; Joana Santos 1 ; Sebastien Tordo 1 ; Elise Vernet 1 ; Roberto Ragazzoni 2 ; Carmelo Arcidiacono 2 ; Paolo Bagnara 3 ; Andrea Baruffolo 3 ; Emiliano Diolaiti 4 ; Jacopo Farinato 2 ; Matteo Lombini 2

1 European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching bei München, Germany
2 INAF, Astrophysical Observatory of Arcetri, Largo Enrico Fermi 5, 50125, Florence, Italy
3 INAF, Astronomical Observatory of Padova, Vicolo dell'Osservatorio 5, 35122, Padova, Italy
4 INAF, Astronomical Observatory of Bologna, Via Ranzani 1, 40127, Bologna, Italy
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     title = {MAD: practical implementation of {MCAO} concepts},
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Enrico Marchetti; Roland Brast; Bernard Delabre; Rob Donaldson; Enrico Fedrigo; Christoph Frank; Norbert Hubin; Johann Kolb; Miska Le Louarn; Jean-Louis Lizon; Sylvain Oberti; Fernando Quirós-Pacheco; Roland Reiss; Joana Santos; Sebastien Tordo; Elise Vernet; Roberto Ragazzoni; Carmelo Arcidiacono; Paolo Bagnara; Andrea Baruffolo; Emiliano Diolaiti; Jacopo Farinato; Matteo Lombini. MAD: practical implementation of MCAO concepts. Comptes Rendus. Physique, Volume 6 (2005) no. 10, pp. 1118-1128. doi : 10.1016/j.crhy.2005.11.002. https://comptes-rendus.academie-sciences.fr/physique/articles/10.1016/j.crhy.2005.11.002/

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