activity
19992009
most citedSystematics in the X-ray Cluster Mass Estimators

311 citations · 1.3k across the 17 of their papers we have counts for

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Showing 2004Show all

7 papers · 1 filter

astro-ph2004

Simulating the Soft X-ray excess in clusters of galaxies

L. -M. Cheng, S. Borgani, P. Tozzi +7

The detection of excess of soft X-ray or Extreme Ultraviolet (EUV) radiation, above the thermal contribution from the hot intracluster medium (ICM), has been a controversial subjec…

astro-ph2004

Mismatch between X-ray and emission-weighted temperatures in galaxy clusters: cosmological implications

E. Rasia, P. Mazzotta, S. Borgani +5

The thermal properties of hydrodynamical simulations of galaxy clusters are usually compared to observations by relying on the emission-weighted temperature T_ew, instead of on the…

astro-ph2004

Voids in a CDM Universe

Joerg M. Colberg, Ravi K. Sheth, Antonaldo Diaferio +2

We study the formation and evolution of voids in the dark matter distribution using various simulations of the popular Cold Dark Matter cosmogony. We identify voids by requirin…

astro-ph2004

Evolution at z>0.5 of the X-ray properties of simulated galaxy clusters: comparison with the observational constraints

S. Ettori, S. Borgani, L. Moscardini +7

(ABRIDGED) We analyze the X-ray properties of a sample of local and high redshift galaxy clusters extracted from a large cosmological hydrodynamical simulation. This simulation has…

astro-ph2004

The Diffuse Light in Simulations of Galaxy Clusters

G. Murante, M. Arnaboldi, O. Gerhard +8

We study the properties of the diffuse light in galaxy clusters forming in a large hydrodynamical cosmological simulation of the Lambda-CDM cosmology. The simulation includes a mod…

astro-ph2004

Measuring cluster peculiar velocities with the Sunyaev-Zeldovich effects: scaling relations and systematics

A. Diaferio, S. Borgani, L. Moscardini +6

The fluctuations in the Cosmic Microwave Background (CMB) intensity due to the Sunyaev-Zeldovich (SZ) effect are the sum of a thermal and a kinetic contribution. Separating the two…