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EAGLE Spectroscopy of Resolved Stellar Populations Beyond the Local Group

Published online by Cambridge University Press:  13 April 2010

Chris Evans ,
Yanbin Yang ,
Mathieu Puech ,
Matthew Lehnert ,
Michael Barker ,
Annette Ferguson ,
Jean-Gabriel Cuby ,
Simon Morris ,
Gérard Rousset  and
François Assémat
...Show all authors
Chris Evans
Affiliation:
UK ATC, Royal Observatory Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, UK email: chris.evans@stfc.ac.uk
Yanbin Yang
Affiliation:
GEPI, Observatoire de Paris, 5 Place Jules Janssen, 92195 Meudon Cedex, France
Mathieu Puech
Affiliation:
GEPI, Observatoire de Paris, 5 Place Jules Janssen, 92195 Meudon Cedex, France
Matthew Lehnert
Affiliation:
GEPI, Observatoire de Paris, 5 Place Jules Janssen, 92195 Meudon Cedex, France
Michael Barker
Affiliation:
IfA, Royal Observatory Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, UK
Annette Ferguson
Affiliation:
IfA, Royal Observatory Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, UK
Jean-Gabriel Cuby
Affiliation:
LAM, OAMP, 38 rue Frédéric Joliot Curie, 13388 Marseille Cedex 13, France
Simon Morris
Affiliation:
Department of Physics, Durham University, South Road, Durham, DH1 3LE, UK
Gérard Rousset
Affiliation:
LESIA, Observatoire de Paris, 5 Place Jules Janssen, 92195 Meudon Cedex, France
François Assémat
Affiliation:
LESIA, Observatoire de Paris, 5 Place Jules Janssen, 92195 Meudon Cedex, France
Hector Flores
Affiliation:
GEPI, Observatoire de Paris, 5 Place Jules Janssen, 92195 Meudon Cedex, France
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Abstract

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We give an overview of the science case for spectroscopy of resolved stellar populations beyond the Local Group with the European Extremely Large Telescope (E-ELT). In particular, we present science simulations undertaken as part of the EAGLE Phase A design study for a multi–integral-field-unit, near-infrared spectrograph. EAGLE will exploit the unprecedented primary aperture of the E-ELT to deliver AO-corrected spectroscopy across a large (38.5 arcmin2) field, truly revolutionising our view of stellar populations in the Local Volume.

Keywords

instrumentation: adaptive optics – instrumentation: spectrographs – galaxies: abundances – galaxies: evolution – galaxies: kinematics & dynamics – galaxies: stellar content
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S262: Stellar Populations – Planning for the Next Decade , August 2009 , pp. 299 - 302
Copyright
Copyright © International Astronomical Union 2010

References

Tolstoy, E. et al. , 2004, ApJL, 617, 119CrossRefGoogle Scholar
Chapman, S. et al. , 2006, ApJ, 653, 255Google Scholar
Rejkuba, M. et al. , 2005, ApJ, 631, 262CrossRefGoogle Scholar
de Jong, R. S. et al. , 2007, IAUS241, p503Google Scholar
Dalcanton, J. J. et al. , 2009, ApJS, 183, 67Google Scholar
Assémat, F., Gendron, E., & Hammer, F., 2007, MNRAS, 376, 287Google Scholar
Myers, R. M. et al. , 2008, SPIE, 7015, 6Google Scholar
Puech, M. et al. , 2008, MNRAS, 390, 1089CrossRefGoogle Scholar
Munari, U. & Castelli, F., 2000, A&AS, 141, 141Google Scholar
Sarazin, M., Melnick, J., Navarrete, J., & Lombardi, G., 2008, Msngr, 132, 11Google Scholar