EAGLE Spectroscopy of Resolved Stellar Populations Beyond the Local Group

Sep, 2009
6 pages
e-Print:

Citations per year

200820092010014
Abstract: (arXiv)
Valuable insights into galaxy evolution can be gleaned from studies of resolved stellar populations in the local Universe. Deep photometric surveys have provided tracers of the star-formation histories in galaxies from 0.8-16 Mpc, but without robust chemical abundances and stellar kinematics from spectroscopy, their sub-structures and assembly histories remain hidden from us. In this context, we introduce the EAGLE design study for a multi--integral-field-unit, near-infrared spectrograph for the European Extremely Large Telescope (E-ELT). EAGLE will exploit the unprecedented light-gathering power of the E-ELT to deliver AO-corrected spectroscopy across a large (38.5 sq. arcmin) field, truly revolutionising our view of stellar populations in the Local Volume.
Note:
  • 6 pages, to appear in the proceedings of the AO4ELT conference, held in Paris, 22-26 June 2009
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