Weighting CMB and Galactic synchrotron polarisation
arXiv:astro-ph/0305415 · doi:10.1016/j.newar.2003.07.012
Abstract
We review the present knowledge of the diffuse Galactic synchrotron emission in polarisation. At microwave frequencies, we assess the expected contamination to the CMB polarisation angular power spectrum, for and modes, as expected after the WMAP first year measurements.
6 pages, 4 figures, proc. of the CMBnet workshop, 20-21 Feb. 2003, Oxford, UK
References in corpus (4)
- Detection of Polarization in the Cosmic Microwave Background using DASI
- All-sky astrophysical component separation with Fast Independent Component Analysis (FastICA)
- Towards a model of full-sky Galactic synchrotron intensity and linear polarisation: a re-analysis of the Parkes data
- The nature of the E-B decomposition of CMB polarization