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EAGLE: A MOAO fed multi-IFU NIR workhorse for E-ELT

Authors :
Emmanuel Hugot
Peter Hastings
Mark Swinbank
Simon L. Morris
Chris Evans
Richard M. Myers
Nigel Dipper
Damien Gratadour
David Le Mignant
I. Bryson
Clélia Robert
Niraj Welikala
Vincent Lebrun
Pascal Vola
Matthew D. Lehnert
Jean-Luc Gimenez
Fabrice Madec
William Taylor
Martyn Wells
Philippe Laporte
Tim Morris
Mathieu Cohen
Sébastien Vivès
G. Talbot
Benoit Neichel
Jean-Gabriel Cuby
Stephen Beard
Hermine Schnetler
Gérard Rousset
Eric Gendron
P. Jagourel
Zoltan Hubert
P. Parr-Burman
Marc Ferrari
François Vidal
Thierry Fusco
Jean-Philippe Amans
Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA)
Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Pôle Astronomie du LESIA
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Source :
Proceedings of the SPIE, Ground-based and Airborne Instrumentation for Astronomy III, Ground-based and Airborne Instrumentation for Astronomy III, Jun 2010, San Diego, California, United States. pp.2D 1-15, ⟨10.1117/12.856820⟩
Publication Year :
2016

Abstract

EAGLE is an instrument under consideration for the European Extremely Large Telescope (E-ELT). EAGLE will be installed at the Gravity Invariant Focal Station of the E-ELT. The baseline design consists of 20 IFUs deployable over a patrol field of ∼40 arcmin2. Each IFU has an individual field of view of ∼ 1.65″ x 1.65″. While EAGLE can operate with the Adaptive Optics correction delivered by the telescope, its full and unrivaled scientific power will be reached with the added value of its embedded Multi-Object Adaptive Optics System (MOAO). EAGLE will be a unique and efficient facility for spatially-resolved, spectroscopic surveys of high-redshift galaxies and resolved stellar populations. We detail the three main science drivers that have been used to specify the top level science requirements. We then present the baseline design of the instrument at the end of Phase A, and in particular its Adaptive Optics System. We show that the instrument has a readiness level that allows us to proceed directly into phase B, and we indicate how the instrument development is planned. © 2010 Copyright SPIE - The International Society for Optical Engineering.

Details

Language :
English
Database :
OpenAIRE
Journal :
Proceedings of the SPIE, Ground-based and Airborne Instrumentation for Astronomy III, Ground-based and Airborne Instrumentation for Astronomy III, Jun 2010, San Diego, California, United States. pp.2D 1-15, ⟨10.1117/12.856820⟩
Accession number :
edsair.doi.dedup.....2b5a9c7395d29a4ccf5ac1be71318b1c
Full Text :
https://doi.org/10.1117/12.856820⟩