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most citedProfiles of dark haloes: evolution, scatter, and environment

2.3k citations · 2.5k across the 7 of their papers we have counts for

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7 papers

astro-ph2000

Origin and Destiny of Dark Matter Halos: Cosmological Matter Exchange and Metal Enrichment

Tsafrir S. Kolatt, James S. Bullock, Avishai Dekel +4

[Abridged] We analyze the exchange of dark matter between halos, subhalos, and their environments in a high-resolution cosmological N-body simulation of a Lambda CDM cosmology. At…

astro-ph2000

Interaction rates of dark-matter halos and subhalos

Tsafrir S. Kolatt, James S. Bullock, Yair Sigad +4

[Abridged] The interaction rates of dark-matter halos and subhalos, are computed using high-resolution cosmological N-body simulations of the Lambda-CDM model. Although the number…

astro-ph2000★ 2 cited

Velocity and Mass Functions of Galactic Halos: Evolution and Environmental Dependence

Yair Sigad, Tsafrir S. Kolatt, James S. Bullock +4

We study the distribution functions of mass and circular velocity for dark matter halos in N-body simulations of the CDM cosmology, addressing redshift and environmental depende…

astro-ph2000★ 43 cited

Measuring the Nonlinear Biasing Function from a Galaxy Redshift Survey

Yair Sigad, Enzo Branchini, Avishai Dekel

We present a simple method for evaluating the nonlinear biasing function of galaxies from a redshift survey. The nonlinear biasing is characterized by the conditional mean of the g…

astro-ph1999★ 2.3k cited

Profiles of dark haloes: evolution, scatter, and environment

James S. Bullock, Tsafrir S. Kolatt, Yair Sigad +5

We study dark-matter halo density profiles in a high-resolution N-body simulation of an LCDM cosmology. Our statistical sample contains ~5000 haloes in the range 10^{11}-10^{14} M_…

astro-ph1999★ 73 cited

Young galaxies: what turns them on?

Tsafrir S. Kolatt, James S. Bullock, Rachel S. Somerville +8

Lyman break galaxies (LBGs) at exhibit number densities and clustering similar to local galaxies; however, their star formation rates (SFRs) are much higher. We ex…