Radio synchrotron emission, its polarization and Faraday rotation of the polarization angle
are powerful tools to study the strength and structure of magnetic fields in galaxies …

Observational results of interstellar and intergalactic magnetic fields are reviewed, including
the fields in supernova remnants and loops, interstellar filaments and clouds, Hii regions …

ABSTRACT A new, much-improved model of the Galactic magnetic field (GMF) is presented.
We use the WMAP7 Galactic synchrotron emission map and more than 40,000 extragalactic …

Here, we describe the Compact Array Broad-band Backend (CABB) and present first results
obtained with the upgraded Australia Telescope Compact Array (ATCA). The 16-fold …

We have re-analyzed the NRAO VLA Sky Survey (NVSS) data to derive rotation measures
(RMs) toward 37,543 polarized radio sources. The resulting catalog of RM values covers the …

We aim to summarize the current state of knowledge regarding Galactic Faraday rotation in
an all-sky map of the Galactic Faraday depth. For this we have assembled the most …

The future of centimetre and metre-wave astronomy lies with the Square Kilometre Array
(SKA), a telescope under development by a consortium of 17 countries that will be 50 times …

The origin and growth of magnetic fields in galaxies is still something of an enigma. It is
generally assumed that seed fields are amplified over time through the dynamo effect,,,, but …

We present a new joint analysis of pulsar dispersion measures and diffuse Hα emission in
the Milky Way, which we use to derive the density, pressure and filling factor of the thick disk …

Most of the visible matter in the Universe is ionized, so that cosmic magnetic fields are quite
easy to generate and due to the lack of magnetic monopoles hard to destroy. Magnetic fields …