Environmental dependence of dark matter halo growth - I. Halo merger rates
- 21 April 2009
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 394 (4) , 1825-1840
- https://doi.org/10.1111/j.1365-2966.2009.14480.x
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- Environmental dependence in the ellipsoidal collapse modelMonthly Notices of the Royal Astronomical Society, 2008
- The nearly universal merger rate of dark matter haloes in ΛCDM cosmologyMonthly Notices of the Royal Astronomical Society, 2008
- Assembly bias in the clustering of dark matter haloesMonthly Notices of the Royal Astronomical Society: Letters, 2007
- The spin and shape of dark matter haloes in the Millennium simulation of a Λ cold dark matter universeMonthly Notices of the Royal Astronomical Society, 2007
- A primer on hierarchical galaxy formation: the semi-analytical approachReports on Progress in Physics, 2006
- The environmental dependence of clustering in hierarchical modelsMonthly Notices of the Royal Astronomical Society, 2005
- The Dependence on Environment of Cold Dark Matter Halo PropertiesThe Astrophysical Journal, 2005
- Cluster evolution as a diagnostic for ΩMonthly Notices of the Royal Astronomical Society, 1996
- Excursion set mass functions for hierarchical Gaussian fluctuationsThe Astrophysical Journal, 1991
- The evolution of large-scale structure in a universe dominated by cold dark matterThe Astrophysical Journal, 1985