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 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 …

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

This is an introduction to Bayesian inference with a focus on hierarchical models and hyper-
parameters. We write primarily for an audience of Bayesian novices, but we hope to provide …

We present the fastemriwaveforms (FEW) package, a collection of tools to build and analyze
extreme mass ratio inspiral (EMRI) waveforms. Here, we expand on [AJK Chua, Phys. Rev …

The Advanced LIGO and Advanced Virgo gravitational-wave (GW) detectors will begin
operation in the coming years, with compact binary coalescence events a likely source for …

The future space mission LISA will observe a wealth of gravitational-wave sources at
millihertz frequencies. Of these, the extreme-mass-ratio inspirals of compact objects into …

We seek to achieve the holy grail of Bayesian inference for gravitational-wave astronomy:
using deep-learning techniques to instantly produce the posterior p (θ| D) for the source …

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 …

We introduce Bilby-mcmc, a Markov chain Monte Carlo sampling algorithm tuned for the
analysis of gravitational waves from merging compact objects. Bilby-mcmc provides a …