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Proceedings Paper

EAGLE MOAO system conceptual design and related technologies
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Paper Abstract

EAGLE is the multi-object spatially-resolved near-IR spectrograph instrument concept for the E-ELT, relying on a distributed Adaptive Optics, so-called Multi Object Adaptive Optics. This paper presents the results of a phase A study. Using 84×84 actuator deformable mirrors, the performed analysis demonstrates that 6 laser guide stars (on an outer ring of 7.2' diameter) and up to 5 natural guide stars of magnitude R < 17, picked-up in a 7.3' diameter patrol field of view, allow us to obtain an overall performance in terms of Ensquared Energy of 35% in a 75×75mas2 resolution element at H band whatever the target direction in the centred 5' science field for median seeing conditions. In terms of sky coverage, the probability to find the 5 natural guide stars is close to 90% at galactic latitudes |b| ~ 60 deg. Several MOAO demonstration activities are also on-going.

Paper Details

Date Published: 28 July 2010
PDF: 11 pages
Proc. SPIE 7736, Adaptive Optics Systems II, 77360S (28 July 2010); doi: 10.1117/12.856586
Show Author Affiliations
G. Rousset, LESIA, CNRS, Observatoire de Paris à Meudon, Univ. Paris Diderot (France)
Groupement d'Intérêt Scientifique PHASE (France)
T. Fusco, ONERA (France)
Groupement d'Intérêt Scientifique PHASE (France)
F. Assemat, LESIA, CNRS, Observatoire de Paris à Meudon, Univ. Paris Diderot (France)
ONERA (France)
Groupement d'Intérêt Scientifique PHASE (France)
E. Gendron, LESIA, CNRS, Observatoire de Paris à Meudon, Univ. Paris Diderot (France)
Groupement d'Intérêt Scientifique PHASE (France)
T. Morris, Durham Univ. (United Kingdom)
C. Robert, ONERA (France)
Groupement d'Intérêt Scientifique PHASE (France)
R. Myers, Durham Univ. (United Kingdom)
M. Cohen, GEPI, CNRS, Observatoire de Paris à Meudon, Univ. Paris Diderot (France)
Groupement d'Intérêt Scientifique PHASE (France)
N. Dipper, Durham Univ. (United Kingdom)
C. Evans, United Kingdom Astronomy Technology Ctr. (United Kingdom)
D. Gratadour, LESIA, CNRS, Observatoire de Paris à Meudon, Univ. Paris Diderot (France)
Groupement d'Intérêt Scientifique PHASE (France)
P. Jagourel, GEPI, CNRS, Observatoire de Paris à Meudon, Univ. Paris Diderot (France)
Groupement d'Intérêt Scientifique PHASE (France)
P. Laporte, GEPI, CNRS, Observatoire de Paris à Meudon, Univ. Paris Diderot (France)
Groupement d'Intérêt Scientifique PHASE (France)
D. Le Mignant, LAM, CNRS, Univ. de Provence (France)
M. Puech, GEPI, CNRS, Observatoire de Paris à Meudon, Univ. Paris Diderot (France)
Groupement d'Intérêt Scientifique PHASE (France)
H. Schnetler, United Kingdom Astronomy Technology Ctr. (United Kingdom)
W. Taylor, United Kingdom Astronomy Technology Ctr. (United Kingdom)
F. Vidal, LESIA, CNRS, Observatoire de Paris à Meudon, Univ. Paris Diderot (France)
Groupement d'Intérêt Scientifique PHASE (France)
J.-G. Cuby, LAM, CNRS, Univ. de Provence (France)
M. Lehnert, GEPI, CNRS, Observatoire de Paris à Meudon, Univ. Paris Diderot (France)
Groupement d'Intérêt Scientifique PHASE (France)
S. Morris, Durham Univ. (United Kingdom)
P. Parr-Burman, United Kingdom Astronomy Technology Ctr. (United Kingdom)


Published in SPIE Proceedings Vol. 7736:
Adaptive Optics Systems II
Brent L. Ellerbroek; Michael Hart; Norbert Hubin; Peter L. Wizinowich, Editor(s)

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