Planck intermediate results. XLII. Large-scale Galactic magnetic fields
Recent models for the large-scale Galactic magnetic fields in the literature have been largely constrained by synchrotron emission and Faraday rotation measures. We use three different but representative models to compare their predicted polarized synchrotron and dust emission with that measured by the Planck satellite. We first update these models
Planck Collaboration et al.
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2016