Constraints on a non-Gaussian χm2 cold dark matter model
Open Access
- 21 December 1999
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 310 (4) , 1111-1118
- https://doi.org/10.1046/j.1365-8711.1999.03033.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 28 references indexed in Scilit:
- The Most Massive Distant Clusters: Determining Ω and σ8The Astrophysical Journal, 1998
- Using Cluster Abundances and Peculiar Velocities to Test the Gaussianity of the Cosmological Density FieldThe Astrophysical Journal, 1998
- Redshift Evolution of Galaxy Cluster DensitiesThe Astrophysical Journal, 1997
- Cluster evolution as a diagnostic for ΩMonthly Notices of the Royal Astronomical Society, 1996
- Properties of the cosmological density distribution functionThe Astrophysical Journal, 1995
- Excursion set mass functions for hierarchical Gaussian fluctuationsThe Astrophysical Journal, 1991
- The evolution of groups of galaxies in the Press-Schechter formalismMonthly Notices of the Royal Astronomical Society, 1991
- Biased clustering in the cold dark matter cosmogonyMonthly Notices of the Royal Astronomical Society, 1989
- Non-Gaussian statistics and the microwave background radiationMonthly Notices of the Royal Astronomical Society, 1987
- The statistics of peaks of Gaussian random fieldsThe Astrophysical Journal, 1986