2009

Breaking the self-averaging properties of spatial galaxy fluctuations in the Sloan Digital Sky Survey - Data Release Six

Labini, Francesco Sylos, Vasilyev, Nikolay L., Baryshev, Yurij V.

Understand

Statistical analyses of finite sample distributions usually assume that fluctuations are self-averaging, i.e.

  • that they are statistically similar in different regions of the given sample volume.
  • By using the scale-length method, we test whether this assumption is satisfied in several samples of the Sloan Digital Sky Survey Data Release Six.
  • We find that the probability density function (PDF) of conditional fluctuations, filtered on large enough spatial scales (i.e., r>30 Mpc/h), shows relevant systematic variations in different sub-volumes of the survey.

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