A Template of Galactic Polarized Synchrotron Emission in the Frame of CMBP Experiments

Details A Template of Galactic Polarized Synchrotron Emission in the Frame of CMBP Experiments A Template of Galactic Polarized Synchrotron Emission in the Frame of CMBP Experiments

Feb 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mim..proc..207b&link_type=abstract

The Magnetized Interstellar Medium, Proceedings of the conference, held in Antalya, Turkey, September 8 - 12, 2003, Eds: B. Uyan

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We present a method to model the polarized Galactic synchrotron emission in the microwave range (20-100 GHz), where this radiation is expected to play the leading role in contaminating Cosmic Microwave Background (CMB) data. Our method is based on real surveys and aims at providing the real spatial distributions of both polarized intensity and polarization angles. Its main features are the modelling of a polarization horizon to determine the polarized intensity and the use of starlight optical data to model the polarization angle pattern. Our template is virtually free of Faraday rotation effects as required at cosmological window frequencies.

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