We present the results of the search for an isotropic stochastic gravitational wave
background (GWB) at nanohertz frequencies using the second data release of the European …

Pulsar timing arrays offer a probe of the low-frequency gravitational wave spectrum (1–100
nHz), which is intimately connected to a number of markers that can uniquely trace the …

We report on Bayesian estimation of the radius, mass, and hot surface regions of the
massive millisecond pulsar PSR J0740+ 6620, conditional on pulse-profile modeling of …

With unparalleled rotational stability, millisecond pulsars (MSPs) serve as ideal laboratories
for numerous astrophysical studies, many of which require precise knowledge of the …

Ultracompact binaries with orbital periods less than a few hours will dominate the
gravitational wave signal in the mHz regime. Until recently, 10 systems were expected to …

We argue that comparison with observations of theoretical models for the velocity
distribution of pulsars must be done directly with the observed quantities, that is parallax and …

We present the results of PSRπ, a large astrometric project targeting radio pulsars using the
Very Long Baseline Array (VLBA). From our astrometric database of 60 pulsars, we have …

ABSTRACT 33 fast radio bursts (FRBs) had been detected by 2018 March. Although the
sample size is still limited, meaningful statistical studies can already be carried out. The …

The aim of this work is to study the imprints that different models for black hole (BH) and
neutron star (NS) formation have on the Galactic distribution of X-ray binaries (XRBs) that …

We report a spectroscopic search for hypervelocity white dwarfs (WDs) that are runaways
from Type Ia supernovae (SNe Ia) and related thermonuclear explosions. Candidates are …