972 citations · 9.1k across the 146 of their papers we have counts for
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Hot and Cooled baryons in SPH simulations of galaxy clusters: physics and numerics
S. Borgani, K. Dolag, G. Murante +7
We discuss an extended set of Tree+SPH simulations of galaxy clusters, with the goal of investigating the interplay between numerical resolution effects and star-formation/feedback…
Angular diameter distance estimates from the Sunyaev-Zel'dovich effect in hydrodynamical cluster simulations
S. Ameglio, S. Borgani, A. Diaferio +1
The angular-diameter distance D_A of a galaxy cluster can be measuread by combining its X-ray emission with the cosmic microwave background fluctution due to the Sunyaev-Zeldovich…
Properties of the diffuse X-ray background in a high-resolution hydrodynamical simulation
M. Roncarelli, L. Moscardini, P. Tozzi +5
We study the properties of the diffuse X-ray background by using the results of a cosmological hydrodynamical simulation of the concordance LambdaCDM model. The simulation follows…
CAIRNS: The Cluster And Infall Region Nearby Survey III. Environmental Dependence of H-alpha Properties of Galaxies
Kenneth Rines, Margaret J. Geller, Michael J. Kurtz +1
We investigate the environmental dependence of star formation in cluster virial regions and infall regions as part of CAIRNS (Cluster And Infall Region Nearby Survey), a large spec…
Caustic and Weak Lensing Estimators of Galaxy Cluster Masses
Antonaldo Diaferio, Margaret J. Geller, Kenneth J. Rines
There are only two methods for estimating the mass distribution in the outer regions of galaxy clusters, where virial equilibrium does not hold: weak gravitational lensing and iden…