학술논문

The WiggleZ Dark Energy Survey: the transition to large-scale cosmic homogeneity
Document Type
Working Paper
Source
Mon.Not.Roy.Astron.Soc.425:116-134,2012
Subject
Astrophysics - Cosmology and Nongalactic Astrophysics
Language
Abstract
We 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(Comment: 21 pages, 16 figures, accepted for publication in MNRAS