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25 April 2024
 
  » arxiv » 1205.6812

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The WiggleZ Dark Energy Survey: the transition to large-scale cosmic homogeneity
Morag Scrimgeour ; Tamara Davis ; Chris Blake ; J. Berian James ; Gregory Poole ; Lister Staveley-Smith ; Sarah Brough ; Matthew Colless ; Carlos Contreras ; Warrick Couch ; Scott Croom ; Darren Croton ; Michael J. Drinkwater ; Karl Forster ; David Gilbank ; Mike Gladders ; Karl Glazebrook ; Ben Jelliffe ; Russell J. Jurek ; I-hui Li ; Barry Madore ; Chris Martin ; Kevin Pimbblet ; Michael Pracy ; Rob Sharp ; Emily Wisnioski ; David Woods ; Ted Wyder ; Howard Yee ;
Date 30 May 2012
AbstractWe have made the largest-volume measurement to date of the transition to large-scale homogeneity in the distribution of galaxies. We use the WiggleZ survey, a spectroscopic survey of over 200,000 blue galaxies in a cosmic volume of ~1 (Gpc/h)^3. A new method of defining the ’homogeneity scale’ is presented, which is more robust than methods previously used in the literature, and which can be easily compared between different surveys. Due to the large cosmic depth of WiggleZ (up to z=1) we are able to make the first measurement of the transition to homogeneity over a range of cosmic epochs. The mean number of galaxies N(<r) in spheres of comoving radius r is proportional to r^3 within 1%, or equivalently the fractal dimension of the sample is within 1% of D_2=3, at radii larger than 71 pm 8 Mpc/h at z~0.2, 70 pm 5 Mpc/h at z~0.4, 81 pm 5 Mpc/h at z~0.6, and 75 pm 4 Mpc/h at z~0.8. We demonstrate the robustness of our results against selection function effects, using a LCDM N-body simulation and a suite of inhomogeneous fractal distributions. The results are in excellent agreement with both the LCDM N-body simulation and an analytical LCDM prediction. We can exclude a fractal distribution with fractal dimension below D_2=2.97 on scales from ~80 Mpc/h up to the largest scales probed by our measurement, ~300 Mpc/h, at 99.99% confidence.
Source arXiv, 1205.6812
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