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19972005
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astro-ph2005

project: III. Gas mass fraction shape in high redshift clusters

Rachida Sadat, Alain Blanchard, Sebastien C. Vauclair +10

We study the gas mass fraction, behavior in project. The typical shape of high redshift galaxy clusters follows the global shape inf…

astro-ph2004

The CLEF-SSH simulation project

A. C. da Silva, S. T. Kay, N. Aghanim +5

The CLEF-SSH simulation project is an international collaboration, involving the IAS, LATT and the University of Sussex, to produce large hydrodynamic simulations of large-scale st…

astro-ph2001

Cosmological Parameter Estimation from CMB and X-ray clusters

M. Douspis, A. Blanchard, R. Sadat +1

We present the results of a combined analysis of cosmic microwave background (CMB) and X-ray galaxy clusters baryon fraction to deduce constraints over 6 in flationnary cosmologica…

astro-ph2001

The baryon fraction in X-Rays galaxy clusters revisited

R. Sadat, A. Blanchard, M. Douspis

One of the most direct way to constrain the matter density of the universe is to measure the baryon content in X-Rays clusters of galaxies. Typical value of the mean gas mass…

astro-ph2001

The XMM-Newton Project

J. G. Bartlett, N. Aghanim, M. Arnaud +16

The abundance of high-redshift galaxy clusters depends sensitively on the matter density $\OmM$ and, to a lesser extent, on the cosmological constant . Measurements of this abun…

astro-ph2000

The Baryon Content of Groups and Clusters of Galaxies

H. Roussel, R. Sadat, A. Blanchard

We have analyzed the properties of a sample of 33 groups and clusters of galaxies and examine the baryon content to check for trends over a decade in temperature down to 1 keV. We…