Modelling the two-point correlation function of galaxy clusters in the Sloan Digital Sky Survey
Open Access
- 11 April 2004
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 349 (3) , 882-888
- https://doi.org/10.1111/j.1365-2966.2004.07559.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 40 references indexed in Scilit:
- Galaxy Bias in Quintessence Cosmological ModelsThe Astrophysical Journal, 2003
- Cosmological Evolution of Linear BiasThe Astrophysical Journal, 2001
- The nature of galaxy bias and clusteringMonthly Notices of the Royal Astronomical Society, 2000
- Cosmological constraints from the clustering properties of the X-ray Brightest Abell-type Cluster sampleMonthly Notices of the Royal Astronomical Society, 1999
- Correlation Length of X‐Ray–Brightest Abell ClustersThe Astrophysical Journal, 1998
- Reconstructing Positions and Peculiar Velocities of Galaxy Clusters within 25,000 Kilometers per Second: The Cluster Real Space DipoleThe Astrophysical Journal, 1996
- The cluster correlation function - Consistent results from an automated surveyThe Astrophysical Journal, 1992
- The statistics of peaks of Gaussian random fieldsThe Astrophysical Journal, 1986
- Are superclusters correlated on a very large scale?The Astrophysical Journal, 1986
- The spatial correlation function of rich clusters of galaxiesThe Astrophysical Journal, 1983