We summarize our current knowledge of neutron-star masses and radii. Recent
instrumentation and computational advances have resulted in a rapid increase in the …

Evidence for a low-frequency stochastic gravitational-wave background has recently been
reported based on analyses of pulsar timing array data. The most likely source of such a …

Despite its importance to our understanding of physics at supranuclear densities, the
equation of state (EoS) of matter deep within neutron stars remains poorly understood …

We present high-precision timing data over time spans of up to 11 years for 45 millisecond
pulsars observed as part of the North American Nanohertz Observatory for Gravitational …

The discovery of a repeating fast radio burst (FRB) source,, FRB 121102, eliminated models
involving cataclysmic events for this source. No other repeating FRB has hitherto been …

In this paper, we describe the International Pulsar Timing Array second data release, which
includes recent pulsar timing data obtained by three regional consortia: the European Pulsar …

Discovery of pulsars is one of the main goals for large radio telescopes. The Five-hundred-
meter Aperture Spherical radio Telescope (FAST), that incorporates an L-band 19-beam …

The highly stable spin of neutron stars can be exploited for a variety of (astro) physical
investigations. In particular, arrays of pulsars with rotational periods of the order of …

Improving survey specifications are causing an exponential rise in pulsar candidate
numbers and data volumes. We study the candidate filters used to mitigate these problems …

We report on the high-precision timing of 42 radio millisecond pulsars (MSPs) observed by
the European Pulsar Timing Array (EPTA). This EPTA Data Release 1.0 extends up to mid …