Galactic synchrotron versus CMB polarized signal in the radiowavelength region

Details Galactic synchrotron versus CMB polarized signal in the radiowavelength region Galactic synchrotron versus CMB polarized signal in the radiowavelength region

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..586..184t&link_type=abstract

RELATIVISTIC ASTROPHYSICS: 20th Texas Symposium. AIP Conference Proceedings, Volume 586, pp. 184-189 (2001).

Computer Science

Databases

2

Background Radiations, Radiation Mechanisms, Polarization, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc.

Scientific paper

Galactic synchrotron will be an important contaminant for forthcoming experiments on CMB polarization. We investigate the angular power spectra of polarized Galactic synchrotron in several surveys (Parkes at 2.4 GHz, Effelsberg at 2.7 GHz and 1.4 GHz), showing that partial sky coverage analysis may lead to largely different results. Reasonable extrapolations to tens of GHz allow us to find a region in the (v,l) plane where the CMB polarized signal is expected to prevail largely. .

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