B-Mode contamination by synchrotron emission from 3-years WMAP data
E. Carretti, G. Bernardi, S. Cortiglioni

TL;DR
This study assesses Galactic synchrotron contamination in the lowest emission sky regions using WMAP data, showing these areas could enable detection of primordial B-mode signals at low tensor-to-scalar ratios, aiding inflationary research.
Contribution
It provides the first comprehensive analysis of synchrotron contamination in the lowest emission regions, demonstrating their potential for primordial B-mode detection.
Findings
Synchrotron emission can mimic B-mode signals for T/S ratios of 10^{-3} to 10^{-2} at 70 GHz.
Lowest emission regions have less contamination than previously estimated for high Galactic latitudes.
These regions could allow direct measurement of T/S ~ 10^{-3}, aiding inflationary studies.
Abstract
We study the contamination of the B-mode of the Cosmic Microwave Background Polarization (CMBP) by Galactic synchrotron in the lowest emission regions of the sky. The 22.8-GHz polarization map of the 3-years WMAP data release is used to identify and analyse such regions. Two areas are selected with signal-to-noise ratio S/N<2 and S/N<3, covering ~16% and ~26% fraction of the sky, respectively. The polarization power spectra of these two areas are dominated by the sky signal on large angular scales (multipoles l < 15), while the noise prevails on degree scales. Angular extrapolations show that the synchrotron emission competes with the CMBP B-mode signal for tensor-to-scalar perturbation power ratio -- at 70-GHz in the 16% lowest emission sky (S/N<2 area). These values worsen by a factor ~5 in the S/N<3 region. The novelty is that our estimates regard the whole…
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Taxonomy
TopicsCosmology and Gravitation Theories · Radio Astronomy Observations and Technology · Geophysics and Gravity Measurements
