The discovery of radio pulsars over a half century ago was a seminal moment in astronomy.
It demonstrated the existence of neutron stars, gave a powerful observational tool to study …

Constraining dynamo theories of magnetic field origin by observation is indispensable but
challenging, in part because the basic quantities measured by observers and predicted by …

The radio-emitting neutron star population encompasses objects with spin periods ranging
from milliseconds to tens of seconds. As they age and spin more slowly, their radio emission …

The polarization of fast radio bursts (FRBs), which are bright astronomical transient
phenomena, contains information about their environments. Using wide-band observations …

Fast radio bursts are millisecond-duration, extragalactic radio flashes of unknown physical
origin,,. The only known repeating fast radio burst source,,—FRB 121102—has been …

Fast radio bursts are bright, unresolved, non-repeating, broadband, millisecond flashes,
found primarily at high Galactic latitudes, with dispersion measures much larger than …

We compute and investigate four types of imprint of a stochastic background of primordial
magnetic fields (PMFs) on the cosmic microwave background (CMB) anisotropies: the …

We report on the discovery and analysis of bursts from nine new repeating fast radio burst
(FRB) sources found using the Canadian Hydrogen Intensity Mapping Experiment (CHIME) …

Aims. This work provides an update to existing reconstructions of the Galactic Faraday
rotation sky by processing almost all Faraday rotation data sets available at the end of the …

Combining high time and frequency resolution full-polarization spectra of fast radio bursts
(FRBs) with knowledge of their host galaxy properties provides an opportunity to study both …