A marked correlation function analysis of halo formation times in the Millennium Simulation
- 11 April 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 367 (3) , 1039-1049
- https://doi.org/10.1111/j.1365-2966.2006.10022.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 42 references indexed in Scilit:
- Cosmology and the Halo Occupation Distribution from Small‐Scale Galaxy Clustering in the Sloan Digital Sky SurveyThe Astrophysical Journal, 2005
- Galaxy ecology: groups and low-density environments in the SDSS and 2dFGRSMonthly Notices of the Royal Astronomical Society, 2004
- The Halo Occupation Distribution and the Physics of Galaxy FormationThe Astrophysical Journal, 2003
- The Halo Occupation Distribution: Toward an Empirical Determination of the Relation between Galaxies and MassThe Astrophysical Journal, 2002
- Luminosity‐ and Morphology‐dependent Clustering of GalaxiesThe Astrophysical Journal, 2000
- A recipe for galaxy formationMonthly Notices of the Royal Astronomical Society, 1994
- 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
- The statistics of peaks of Gaussian random fieldsThe Astrophysical Journal, 1986