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19932026
most citedMeasuring and Modelling the Redshift Evolution of Clustering: the Hubble Deep Field North

986 citations · 20.2k across the 394 of their papers we have counts for

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Showing 2003Show all

10 papers · 1 filter

astro-ph2003★ 110 cited

The impact of cluster mergers on arc statistics

Elena Torri, Massimo Meneghetti, Matthias Bartelmann +3

We study the impact of merger events on the strong lensing properties of galaxy clusters. Previous lensing simulations were not able to resolve dynamical time scales of cluster len…

astro-ph2003★ 380 cited

X-ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulation

S. Borgani, G. Murante, V. Springel +6

We present results on the X-ray properties of clusters and groups of galaxies, extracted from a large hydrodynamical simulation. We used the GADGET code to simulate a LambdaCDM mod…

astro-ph2003★ 329 cited

Numerical study of halo concentrations in dark-energy cosmologies

Klaus Dolag, Matthias Bartelmann, Francesca Perrotta +4

We study the concentration parameters, their mass dependence and redshift evolution, of dark-matter halos in different dark-energy cosmologies with constant and time-variable equat…

astro-ph2003★ 279 cited

A dynamical model for the distribution of dark matter and gas in galaxy clusters

Elena Rasia, Giuseppe Tormen, Lauro Moscardini

Using high-resolution non-radiative hydrodynamic simulations of galaxy clusters we obtain simple analytic formulae for DM and gas distribution in the spherical approximation. We de…

astro-ph2003★ 36 cited

Constraints on extended quintessence from high-redshift Supernovae

Paolo Caresia, Sabino Matarrese, Lauro Moscardini

We obtain constraints on quintessence models from magnitude-redshift measurements of 176 type Ia Supernovae. The considered quintessence models are ordinary quintessence, with Ratr…

astro-ph2003★ 71 cited

High-Resolution Simulations of Cosmic Microwave Background non-Gaussian Maps in Spherical Coordinates

Michele Liguori, Sabino Matarrese, Lauro Moscardini

We describe a new numerical algorithm to obtain high-resolution simulated maps of the Cosmic Microwave Background (CMB), for a broad class of non-Gaussian models. The kind of non-G…