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Component separation methods for the Planck mission
S. M. Leach, J. -F. Cardoso, C. Baccigalupi +27
The Planck satellite will map the full sky at nine frequencies from 30 to 857 GHz. The CMB intensity and polarization that are its prime targets are contaminated by foreground emis…
A reassessment of the evidence of the Integrated Sachs-Wolfe effect through the WMAP-NVSS correlation
A. Raccanelli, A. Bonaldi, M. Negrello +3
We reassess the estimate of the cross-correlation of the spatial distribution of the NRAO VLA Sky Survey (NVSS) radio sources with that of Cosmic Microwave Background (CMB) anisotr…
Sunyaev-Zel'dovich profiles and scaling relations: modelling effects and observational biases
A. Bonaldi, G. Tormen, K. Dolag +1
We use high-resolution hydrodynamic re-simulations to investigate the properties of the thermal Sunyaev-Zel'dovich (SZ) effect from galaxy clusters. We compare results obtained usi…
Simulating the physical properties of dark matter and gas inside the cosmic web
K. Dolag, M. Meneghetti, L. Moscardini +2
Using the results of a high-resolution, cosmological hydrodynamical re-simulation of a supercluster-like region we investigate the physical properties of the gas located along the…