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20092015
most citedHaloes gone MAD: The Halo-Finder Comparison Project

422 citations · 1.1k across the 10 of their papers we have counts for

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7 papers · 1 filter

astro-ph.CO2015★ 20 cited

Novel Adaptive softening for collisionless N-body simulations: Eliminating spurious halos

Alexander Hobbs, Justin Read, Oscar Agertz +2

We describe a NOVel form of Adaptive softening (NovA) for collisionless -body simulations, implemented in the Ramses adaptive mesh refinement code. We introduce a refinement cri…

astro-ph.CO2012★ 29 cited

On the orbital and internal evolution of cluster galaxies

Francesca Iannuzzi, Klaus Dolag

Galaxies inhabiting a cluster environment experience significant evolution in their orbital motions throughout time; this is accompanied by changes in the anisotropy parameter, mea…

astro-ph.CO2011★ 31 cited

Adaptive gravitational softening in GADGET

Francesca Iannuzzi, Klaus Dolag

Cosmological simulations of structure formation follow the collisionless evolution of dark matter starting from a nearly homogeneous field at early times down to the highly cluster…

astro-ph.CO2011★ 32 cited

Baryon history and cosmic star formation in non-Gaussian cosmological models: numerical simulations

Umberto Maio, Francesca Iannuzzi

We present the first numerical, N-body, hydrodynamical, chemical simulations of cosmic structure formation in the framework of non-Gaussian models. We study the impact of primordia…

astro-ph.CO2011★ 422 cited

Haloes gone MAD: The Halo-Finder Comparison Project

Alexander Knebe, Steffen R. Knollmann, Stuart I. Muldrew +34

[abridged] We present a detailed comparison of fundamental dark matter halo properties retrieved by a substantial number of different halo finders. These codes span a wide range of…

astro-ph.CO2009★ 22 cited

Imprints of primordial non-Gaussianities in X-ray and SZ signals from galaxy clusters

M. Roncarelli, L. Moscardini, E. Branchini +4

Several inflationary models predict the possibility that the primordial perturbations of the density field may contain a degree of non-Gaussianity which would influence the subsequ…

astro-ph.CO2009★ 159 cited

Large-scale non-Gaussian mass function and halo bias: tests on N-body simulations

M. Grossi, L. Verde, C. Carbone +5

The description of the abundance and clustering of halos for non-Gaussian initial conditions has recently received renewed interest, motivated by the forthcoming large galaxy and c…