We employ the formalism developed in [1] and [2] to study the prospect of detecting an
anisotropic Stochastic Gravitational Wave Background (SGWB) with the Laser Interferometer …

Pulsar timing arrays (PTAs) are ensembles of regularly observed millisecond pulsars timed
to high precision. Each pulsar in an array could be affected by a suite of noise processes …

We examine expected effective spin () and orbital eccentricity () correlations for a population
of observable equal-mass massive black hole binaries (MBHBs) with total redshifted mass …

In an accompanying publication, the MeerKAT Pulsar Timing Array (MPTA) Collaboration
reports tentative evidence for the presence of a stochastic gravitational wave background …

In this work, we investigated the presence of strictly periodic, as well as quasi-periodic
signals, in the timing of the 25 millisecond pulsars (MSPs) from the European Pulsar Timing …

Propagation effects are one of the main sources of noise in high-precision pulsar timing. For
pulsars below an ecliptic latitude of 5°, the ionized plasma in the solar wind can introduce …

ABSTRACT Evaluating the Kirchhoff–Fresnel diffraction integral is essential in studying
wave effects in astrophysical lensing, but is often intractable because of the highly oscillatory …

Recent results from pulsar timing arrays (PTAs) show evidence for a gravitational wave
background (GWB) consistent with a population of unresolved supermassive black hole …

Pulsar timing, ie the analysis of the arrival times of pulses from a pulsar, is a powerful tool in
modern astrophysics. It allows us to measure the time delays of an electromagnetic signal …

The Laser Interferometer Space Antenna (LISA) is a future ESA-led space-based
observatory to explore the gravitational universe in the frequency band between 10^-4 Hz …