A host of new low-frequency radio telescopes seek to measure the 21 cm transition of
neutral hydrogen from the early universe. These telescopes have the potential to directly …

ABSTRACT A Faraday rotation measure (RM) catalogue, or RM Grid, is a valuable resource
for the study of cosmic magnetism. Using the second data release (DR2) from the LOFAR …

The Murchison Widefield Array (MWA), located in Western Australia, is one of the low-
frequency precursors of the international Square Kilometre Array (SKA) project. In addition to …

We study the impact of sky-based calibration errors from source mismodelling on 21 cm
power spectrum measurements with an interferometer and propose a method for …

We present results from the first all-sky radio survey in circular polarization. The survey uses
the Murchison Widefield Array (MWA) to cover 30 900 sq deg, over declinations south of+ …

Magnetic fields in the ionized medium of the disk and halo of the Milky Way impose Faraday
rotation on linearly polarized radio emission. We compare two surveys map** the Galactic …

ABSTRACT Global (ie sky-averaged) 21-cm signal experiments can measure the evolution
of the Universe from the cosmic dawn to the epoch of reionization (EoR). These …

Cosmological simulations predict that an intergalactic magnetic field (IGMF) pervades the
large scale structure (LSS) of the Universe. Measuring the IGMF is important to determine its …

Magnetic fields pervade the interstellar medium (ISM), but are difficult to detect and
characterize. The new generation of low-frequency radio telescopes, such as the Low …

We present techniques developed to calibrate and correct Murchison Widefield Array low-
frequency (72–300 MHz) radio observations for polarimetry. The extremely wide field-of …