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Recently, it has been recognised that very large spectroscopic surveys(several million spectra) are required to advance our understanding of DarkEnergy (via baryonic wiggles) and the detailed history of our Local Group ofgalaxies (via Galactic Archeology or near-field cosmology). In this paper Imake a preliminary exploration of how this might be done by putting a widefield, optical, prime-focus fibre-fed spectroscopic facility on one of theVLT's UTs.

Very Large Spectroscopic Surveys with the VLT