8 pages, 9 figuresInternational audienceAims.We study the dependence of the halo abundance function (AF) on different environments in a whole-sky $\Lambda$CDM light-cone halo catalogue extending to z 0.45), which probably implies a significant and recent evolution of the isolation status of the most isolated and most massive haloes
Using a series of high-resolution N-body simulations of the concordance cosmology we investigate how...
We investigate the dependence of the mass function of dark-matter haloes on their environment within...
Cosmological models in which dark matter consists of cold elementary particles predict that the dark...
Aims. We study the dependence of the halo abundance function (AF) on different environments in a who...
International audienceAims. We study the dependence of the halo abundance function (AF) on different...
International audienceAims. We study the dependence of the halo abundance function (AF) on different...
International audienceAims. We study the dependence of the halo abundance function (AF) on different...
We use large N-body simulations of dissipationless gravitational clustering in cold dark matter (CDM...
We discuss the impact of the cosmological environment on the evolution of dark matter halos using a ...
We introduce a new model of the evolution of the concentration of dark matter halos, c(t). For indiv...
We use a high-resolution ΛCDM numerical simulation to calculate the mass function of dark matter hal...
We study the environmental dependence of the formation history of dark matter haloes in a large dark...
We study the relationship between dark-matter haloes and matter in the MIP N-body simu-lation ensemb...
A basic assumption in the current halo-occupation model is that the properties of a galaxy depend on...
We combine data from a number of N-body simulations to predict the abundance of dark haloes in cold ...
Using a series of high-resolution N-body simulations of the concordance cosmology we investigate how...
We investigate the dependence of the mass function of dark-matter haloes on their environment within...
Cosmological models in which dark matter consists of cold elementary particles predict that the dark...
Aims. We study the dependence of the halo abundance function (AF) on different environments in a who...
International audienceAims. We study the dependence of the halo abundance function (AF) on different...
International audienceAims. We study the dependence of the halo abundance function (AF) on different...
International audienceAims. We study the dependence of the halo abundance function (AF) on different...
We use large N-body simulations of dissipationless gravitational clustering in cold dark matter (CDM...
We discuss the impact of the cosmological environment on the evolution of dark matter halos using a ...
We introduce a new model of the evolution of the concentration of dark matter halos, c(t). For indiv...
We use a high-resolution ΛCDM numerical simulation to calculate the mass function of dark matter hal...
We study the environmental dependence of the formation history of dark matter haloes in a large dark...
We study the relationship between dark-matter haloes and matter in the MIP N-body simu-lation ensemb...
A basic assumption in the current halo-occupation model is that the properties of a galaxy depend on...
We combine data from a number of N-body simulations to predict the abundance of dark haloes in cold ...
Using a series of high-resolution N-body simulations of the concordance cosmology we investigate how...
We investigate the dependence of the mass function of dark-matter haloes on their environment within...
Cosmological models in which dark matter consists of cold elementary particles predict that the dark...