Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-10-03
Astron.Astrophys.500:657-665,2009
Astronomy and Astrophysics
Astrophysics
10 pages. Published version
Scientific paper
10.1051/0004-6361/200811077
We use measurements of cosmic shear from CFHTLS, combined with WMAP-5 cosmic microwave background anisotropy data, baryonic acoustic oscillations from SDSS and 2dFGRS and supernovae data from SNLS and Gold-set, to constrain the neutrino mass. We obtain a 95% confidence level upper limit of 0.54 eV for the sum of the neutrino masses, and a lower limit of 0.03 eV. The preference for massive neutrinos vanishes when shear-measurement systematics are included in the analysis.
Fu Li-ping
Kilbinger Martin
Schimd Carlo
Tereno Ismael
Uzan Jean-Philippe
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