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Science Requirements for EAGLE for the E-ELT
C. J. Evans 1, M. D. Lehnert 2, J. -G. Cuby 3, 4, S. L. Morris 5, A. M. Swinbank 5, W. D. Taylor 1, D. M. Alexander 5, N. P. F. Lorente, Y. Clenet 6, T. Paumard 6, 7
(2008-07-18)

We present an overview of the EAGLE science case, which spans spatially-resolved spectroscopy of targets from five key science areas - ranging from studies of heavily-obscured Galactic star clusters, right out to the first galaxies at the highest redshifts. Here we summarise the requirements adopted for study and also evaluate the availability of natural guide stars in example fields, which will impact on the adaptive optics performance and architecture.
1:  Royal Observatory Edinburgh
Royal Observatory Edinburgh
2:  Galaxies, Etoiles, Physique, Instrumentation (GEPI)
CNRS : UMR8111 – INSU – Observatoire de Paris – Université Paris VII - Paris Diderot
3:  European Southern Observatory (ESO)
ESO
4:  Laboratoire d'Astrophysique de Marseille (LAM)
CNRS : UMR6110 – INSU – Université de Provence - Aix-Marseille I
5:  Department of Physics
Durham University
6:  Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA)
CNRS : UMR8109 – INSU – Observatoire de Paris – Université Pierre et Marie Curie (UPMC) - Paris VI – Université Paris VII - Paris Diderot
7:  Institut d'Astrophysique de Paris (IAP)
CNRS : UMR7095 – INSU – Université Pierre et Marie Curie (UPMC) - Paris VI
Physics/Astrophysics/Cosmology and Extra-Galactic Astrophysics
Fulltext link: 
http://fr.arXiv.org/abs/0807.2945