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The Void Probability Function as a Statistical Indicator

Published online by Cambridge University Press:  19 July 2016

Marc Lachièze-Rey  and
Sophie Maurogordato
Marc Lachièze-Rey
Affiliation:
DPh/SAp, CEN Saclay, 91191 Gif sur Yvette Cedex, France
Sophie Maurogordato
Affiliation:
DPh/SAp, CEN Saclay, 91191 Gif sur Yvette Cedex, France

Extract

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Recent results concerning the galaxy distribution at scales < 100 h−1 Mpc (Ho = 100 h kms−1 Mpc−1) show a number of characteristics which cannot be described by conventional statistical models. Correlation functions, for instance, can in no way give account of the presence of voids of the cellular (or spongy) appearance of the local galaxy distribution (M. Geller, this conference). There is clearly a need for new kinds of statistical models and statistical indicators.

Type
CHAPTER IV: The Large Scale Distribution of Galaxies
Information
Symposium - International Astronomical Union , Volume 124: Observational Cosmology , 1987 , pp. 359 - 362
Copyright
Copyright © Reidel 1987 

References

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