activity
19942009
most citedThe velocity function in the local environment from LCDM and LWDM constrained simulations

190 citations · 431 across the 11 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008

Comparison of clustering properties of observed objects and dark matter halos on different mass and spatial scales

A. V. Tikhonov, A. I. Kopylov, S. Gottlober +1

We investigate the large-scale distribution of galaxy clusters taken from several X-ray catalogs. Different statistics of clustering like the conditional correlation function (CCF)…

astro-ph200724 cited

The Future of the Local Large Scale Structure: the roles of Dark Matter and Dark Energy

Yehuda Hoffman, Ofer Lahav, Gustavo Yepes +1

We study the distinct effects of Dark Matter and Dark Energy on the future evolution of nearby large scale structures using constrained N-body simulations. We contrast a model of C…

astro-ph2007100 cited

Shape, spin and baryon fraction of clusters in the MareNostrum Universe

Stefan Gottloeber, Gustavo Yepes

The MareNostrum Universe is one of the largest cosmological SPH simulation done so far. It consists of dark and gas particles in a box of 500 Mpc on a si…

astro-ph1999

A Numerical Study of Galaxy Properties from Cosmological Simulations with Star Formation

G. Yepes, D. Elizondo, Y. Ascasibar

From a set of 3D cosmological simulations which incorporate a self-consistent model of the star-gas interactions, we have been able to obtain a statistically significant sample of…

astro-ph1997

Numerical Simulations of Galaxy Formation: Cooling, Heating, Star Formation

Anatoly Klypin, Stefan Gottlober, Gustavo Yepes

Formation of luminous matter in the Universe is a complicated process, which includes many processes and components. It is the vastly different scales involved in the process (from…

astro-ph1994

The Angular Correlation Function of Galaxies in CDM and CHDM Models

G. Yepes, A. Klypin, A. Campos +1

We estimate the angular correlation function for the standard CDM, tilted CDM and hybrid (CHDM) models, and compare with observations. When compared with the APM observatio…