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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…
CMB data analysis and sparsity
P. Abrial, Y. Moudden, J. -L. Starck +3
The statistical analysis of the soon to come Planck satellite CMB data will help set tighter bounds on major cosmological parameters. On the way, a number of practical difficulties…
FASTLens (FAst STatistics for weak Lensing) : Fast method for Weak Lensing Statistics and map making
S. Pires, J. -L. Starck, A. Amara +3
With increasingly large data sets, weak lensing measurements are able to measure cosmological parameters with ever greater precision. However this increased accuracy also places gr…