The VLT Spectroscopic Program of the SuperNova Legacy Survey

Details The VLT Spectroscopic Program of the SuperNova Legacy Survey The VLT Spectroscopic Program of the SuperNova Legacy Survey

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..342..501b&link_type=abstract

1604-2004: Supernovae as Cosmological Lighthouses, ASP Conference Series, Vol. 342, Proceedings of the conference held 15-19 Jun

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The SuperNova Legacy Survey is a 5 year project aiming at detecting, monitoring and studying several hundreds type Ia supernova up to redshift z=1. Its main scientific motivation is to precisely measure the Dark Energy equation of state. ESO, through the VLT, plays a major role in the spectroscopic follow-up of supernova candidates. A large program has been granted to identify them and to measure their redshift. In this poster, we present preliminary results of the first year of spectroscopic observations with the ESO VLT.
SNLS home page: cfht.hawaii.edu/SNLS

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