The objective of SNLS is to find and study high-redshift supernovae for cosmological applications. It follows in the steps of the original studies that made the surprising discovery of a non-vanishing cosmological constant or, equivalently, a vacuum energy. SNLS strives to refine these original results by measuring the cosmological parameter w, the ratio between the cosmological pressure and energy density, thereby studying the possible time variation of the vacuum energy. Measurements of supernovae at high redshift (of order 1) are complementary to measurments of the Cosmic Microwave Background that correspond to redshifts of order 1000. The two give independent, nearly orthogonal, constraints on the cosmological matter and vacuum densities. Combining the two types of measurements gives a precise determination of the densities.
Dapnia/SPP, LPNHE-Jussieu (Univ Paris6-Paris7), LAM-Marseilles, University of Toronto, University of Victoria
Search for supernovae in deep images (exposure time near one hour) taken with the CFHT (Hawaii) in four fields of 1 deg2. The exposures are taken each month within 10 days of the new Moon.
The redshifts are determined from spectra taken with 8-meter class telescopes (exposure times of order 1 hour).
Photometry: Megacam is set up at CFHT. When first installed, Megacam was the largest CCD camera in the world (40 CCD, 2kx4k= 300 million pixels).
Spectroscopy: done usito 3 8-meter class telescopes: VLT (Chili), Gemini (Chili and Hawaii), Keck (Hawaii)
SNLS is presently the most productive high-redshift supernova program.
Construction of the Megacam camera and data analysis at the SPP.
The first-year data yielded in 2005 a measurement of w to within 10% of the value expected for a cosmological constant. The paper was the third most cited astrophysical paper for that year.
last update : 03-17 00:00:00-2010 (2289)