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Scale dependent non-Gaussianities in the CMB data identified with Minkowski Functionals and Scaling Indices
H. I. Modest, C. Räth, A. J. Banday +6
In order to test for non-Gaussianities with respect to scale-dependencies we use so-called surrogate maps, in which possible phase correlations of the Fourier phases of the origina…
The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths
J. Delabrouille, M. Betoule, J. -B. Melin +39
We present the Planck Sky Model (PSM), a parametric model for the generation of all-sky, few arcminute resolution maps of sky emission at submillimetre to centimetre wavelengths, i…
Sparse component separation for accurate CMB map estimation
J. Bobin, J. -L. Starck, F. Sureau +1
The Cosmological Microwave Background (CMB) is of premier importance for the cosmologists to study the birth of our universe. Unfortunately, most CMB experiments such as COBE, WMAP…
A needlet ILC analysis of WMAP 9-year polarisation data: CMB polarisation power spectra
Soumen Basak, Jacques Delabrouille
We estimate Cosmic Microwave Background (CMB) polarisation power spectra, and temperature-polarisation cross-spectra, from the 9-year data of the Wilkinson Microwave Anisotropy Pro…