Accueil > Séminaires d’Astrophysique > EAGLE - An efficient facility spectrometer for the European Extremely Large Telescope (E-ELT)

 

EAGLE - An efficient facility spectrometer for the European Extremely Large Telescope (E-ELT)

Jean-Gabriel Cuby (LAM, Marseille) — au CESR

Par Francois RINCON - 2/03/2010

 

Séminaires d’Astrophysique

de l’Observatoire Midi-Pyrénées


Séminaire de

Jean-Gabriel Cuby

(LAM, Marseille)

Jeudi 11 Mars 2010 à 11h

CESR


EAGLE - An efficient facility spectrometer for the European Extremely Large Telescope (E-ELT)

EAGLE is an instrument for the European Extremely Large Telescope (E-ELT). It is designed for spectroscopic observations, assisted by Adaptive Optics, of high redshift galaxies and stellar populations at Mpc distances, strongly complementing the capabilities of JWST and ALMA. The 2-yr ESO funded phase A study was completed in the fall of 2009 by a consortium of UK and French institutes. The instrument, as designed, can be built with existing technologies at an affordable cost and manageable risks. We provide a status report of the instrument design and system, and provide performance estimates comparing EAGLE with other space and ground based facilities.

 

 

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Laboratoire Astrophysique de Toulouse - Tarbes (UMR5572)

CNRS (Midi-Pyrénées)

Univ. Paul Sabatier

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