Abstract The Laser Interferometer Space Antenna (LISA) has the potential to reveal wonders
about the fundamental theory of nature at play in the extreme gravity regime, where the …

70 AIM, UMR 7158, CEA/DRF, CNRS, Université Paris Diderot, Irfu/Service d'Astrophysique,
Centre de Saclay, FR-91191 Gif-sur-Yvette, France

We present imrphenomxphm, a phenomenological frequency-domain model for the
gravitational-wave signal emitted by quasicircular precessing binary black holes, which …

We present our current best estimate of the plausible observing scenarios for the Advanced
LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next several years …

Understanding the properties of transient gravitational waves (GWs) and their sources is of
broad interest in physics and astronomy. Bayesian inference is the standard framework for …

Numerical relativity (NR) simulations provide the most accurate binary black hole
gravitational waveforms, but are prohibitively expensive for applications such as parameter …

We present a rapid parameter estimation framework for compact binary coalescence (CBC)
signals observed by the LIGO-Virgo-KAGRA (LVK) detector network. The goal of our …

We develop new strategies to build numerical relativity surrogate models for eccentric binary
black hole systems, which are expected to play an increasingly important role in current and …

Orbital eccentricity is a crucial physical effect to unveil the origin of compact-object binaries
detected by ground-and spaced-based gravitational-wave (GW) observatories. Here, we …

I provide a frequency domain reduced order model (ROM) for the aligned-spin effective-one-
body model “SEOBNRv2” for data analysis with second-and third-generation ground-based …