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Issue A&A
Volume 388, Number 3, June IV 2002
Page(s) 758 - 765
Section Cosmology
DOI http://dx.doi.org/10.1051/0004-6361:20020551



A&A 388, 758-765 (2002)
DOI: 10.1051/0004-6361:20020551

Point field models for the galaxy point pattern

Modelling the singularity of the two-point correlation function
M. Snethlage1, V. J. Martínez2, D. Stoyan3 and E. Saar4

1  Mathematical Department, Silesian University at Opava, Bezrucovo nám. 13, 74601 Opava 1, Czech Republik
    e-mail: Martin.Snethlage@math.slu.cz
2  Observatori Astrònomic, Universitat de València, 46100 Burjassot, Spain
3  Institut für Stochastik, TU Bergakademie Freiberg, Bernhard-von-Cotta-Str. 2, 09596 Freiberg, Germany
    e-mail: stoyan@orion.hrz.tu-freiberg.de
4  Tartu Observatory, Tõravere, 61602, Estonia
    e-mail: saar@aai.ee

(Received 7 December 2001 / Accepted 8 April 2002)

Abstract
There is empirical evidence that the two-point correlation function of the galaxy distribution follows, for small scales, reasonably well a power-law expression $\xi(r)\propto
r^{-\gamma}$ with $\gamma$ between 1.5 and 1.9. Nevertheless, most of the point field models suggested in the literature do not have this property. This paper presents a new class of models, which is produced by modifying point fields commonly used in cosmology to mimic the galaxy distribution, but where $\gamma=2$ is too large. The points are independently and randomly shifted, leading to the desired reduction of the value of $\gamma$.


Key words: galaxies: statistics -- large-scale structure of universe -- methods: statistical

Offprint request: V. J. Martínez, Vicent.Martinez@uv.es




© ESO 2002


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