|
||||||||||||||||||
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. Saar41 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
with
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
is too large. The points
are independently and randomly shifted, leading to the desired
reduction of the value of
.
Key words: galaxies: statistics -- large-scale structure of universe -- methods: statistical
Offprint request: V. J. Martínez, Vicent.Martinez@uv.es
© ESO 2002
| What is OpenURL? |
- If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
- You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
- You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.

BibSonomy
CiteUlike
Connotea
Del.icio.us
Digg
Facebook