High Galactic latitude polarized emission at 1.4 GHz and implications for cosmic microwave background observations
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/358/1/1/3468188/358-1-1.pdf
Reference44 articles.
1. The Linear Polarization of Part of the Northern Sky at 49-cm Wavelength
2. First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Foreground Emission
3. Bernardi G. , 2004, PhD thesis, Universitá di Bologna
4. Polarization Observations in a Low Synchrotron Emission Field at 1.4 GHz
5. A polarized synchrotron template for cosmic microwave background polarization experiments based on WMAP data
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2. Simulations of Galactic polarized synchrotron emission for Epoch of Reionization observations;Monthly Notices of the Royal Astronomical Society;2018-06-05
3. Constraining Polarized Foregrounds for EoR Experiments. II. Polarization Leakage Simulations in the Avoidance Scheme;The Astrophysical Journal;2017-10-10
4. The Fan Region at 1.5 GHz – I. Polarized synchrotron emission extending beyond the Perseus Arm;Monthly Notices of the Royal Astronomical Society;2017-02-16
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