WiggleZ Dark Energy Survey: Cosmological neutrino mass constraint from blue high-redshift galaxies

@article{RiemerSrensen2012WiggleZDE,
  title={WiggleZ Dark Energy Survey: Cosmological neutrino mass constraint from blue high-redshift galaxies},
  author={S. Riemer-S{\o}rensen and C. Blake and D. Parkinson and T. Davis and S. Brough and M. Colless and C. Contreras and W. Couch and S. Croom and D. Croton and M. Drinkwater and K. Forster and D. Gilbank and M. Gladders and K. Glazebrook and Ben Jelliffe and R. Jurek and I. Li and B. Madore and D. Martin and K. Pimbblet and G. Poole and M. Pracy and R. Sharp and E. Wisnioski and D. Woods and T. Wyder and H. Yee},
  journal={Physical Review D},
  year={2012},
  volume={85},
  pages={081101}
}
The absolute neutrino mass scale is currently unknown, but can be constrained by cosmology. The WiggleZ high redshift, star-forming, and blue galaxy sample offers a complementary data set to previous surveys for performing these measurements, with potentially different systematics from nonlinear structure formation, redshift-space distortions, and galaxy bias. We obtain a limit of ∑m_ν<0.60  eV (95% confidence) for WiggleZ+Wilkinson Microwave Anisotropy Probe. Combining with priors on the… Expand
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