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19982004
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Showing 2004 · astro-phShow all

7 papers · 2 filters

astro-ph2004

Clusters of Galaxies: New Results from the CLEF Hydrodynamics Simulation

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

Preliminary results are presented from the CLEF hydrodynamics simulation, a large (N=2(428)^3 particles within a 200 Mpc/h comoving box) simulation of the LCDM cosmology that inclu…

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-ph2004

CMB Quadrupole induced polarisation from clusters and filaments

Guo-Chin Liu, Antonio da Silva, Nabila Aghanim

We present the estimates of the Cosmic Microwave Background (CMB) polarisation power spectrum from galaxy clusters and filaments using hydrodynamical simulations of large scale str…

astro-ph2004

Primordial quadrupole-induced polarisation from filamentary structures and galaxy clusters

Guo Chin Liu, Antonio da Silva, Nabila Aghanim

We present the first computation of the Cosmic Microwave Background (CMB) polarisation power spectrum from galaxy clusters and filaments using hydrodynamical simulations of large s…

astro-ph2004

The distance duality relation from X-ray and SZ observations of clusters

Jean-Philippe Uzan, Nabila Aghanim, Yannick Mellier

X-ray and Sunyaev-Zel'dovich data of clusters of galaxies enable to construct a test of the distance duality relation between the angular and luminosity distances. We argue that su…

astro-ph2004

Separating the kinetic SZ effect from primary CMB fluctuations

O. Forni, N. Aghanim

In the present work, we propose a new method aiming at extracting the kinetic Sunyaev-Zel'dovich (KSZ) temperature fluctuations embedded in the primary anisotropies of the cosmic m…