The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9

@article{Blake2011TheWD,
  title={The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9},
  author={C. Blake and S. Brough and M. Colless and C. Contreras and W. Couch and S. Croom and T. Davis 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 Chris 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={Monthly Notices of the Royal Astronomical Society},
  year={2011},
  volume={415},
  pages={2876-2891}
}
We present precise measurements of the growth rate of cosmic structure for the redshift range 0.1 < z < 0.9, using redshift-space distortions in the galaxy power spectrum of the WiggleZ Dark Energy Survey. Our results, which have a precision of around 10 per cent in four independent redshift bins, are well fitted by a flat Λ cold dark matter (ΛCDM) cosmological model with matter density parameter Ω_m = 0.27. Our analysis hence indicates that this model provides a self-consistent description of… Expand
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