International audienceGravitational waves provide a unique tool for observational astronomy. While the first LIGO–Virgo catalogue of gravitational-wave transients (GWTC-1) contains 11 signals from black hole and neutron star binaries, the number of observations is increasing rapidly as detector sensitivity improves. To extract information from the observed signals, it is imperative to have fast, flexible, and scalable inference techniques. In a previous paper, we introduced bilby: a modular and user-friendly Bayesian inference library adapted to address the needs of gravitational-wave inference. In this work, we demonstrate that bilby produces reliable results for simulated gravitational-wave signals from compact binary mergers, and verify ...
Second-generation interferometric gravitational-wave detectors, such as Advanced LIGO and Advanced V...
Understanding the properties of transient gravitational waves (GWs) and their sources is of broad in...
The coalescence of compact binaries containing neutron stars or black holes is one of the most promi...
International audienceGravitational waves provide a unique tool for observational astronomy. While t...
ABSTRACT Gravitational waves provide a unique tool for observational astronomy. Whi...
Gravitational waves provide a unique tool for observational astronomy. While the first LIGO–Virgo ca...
Gravitational waves provide a unique tool for observational astronomy. While the first LIGO–Virgo ca...
Bayesian parameter estimation is fast becoming the language of gravitational-wave astronomy. It is t...
A major challenge in gravitational-wave astrophysics is the interpretation of observations, which re...
We introduce new modules in the open-source PyCBC gravitational- wave astronomy toolkit that impleme...
The Advanced LIGO and Advanced Virgo gravitational-wave (GW) detectors will begin operation in the c...
The Advanced LIGO and Advanced Virgo gravitational wave (GW) detectors will begin operation in the c...
Detecting gravitational waves is just the start of the story; to understand their nature and the sys...
Third generation (3G) gravitational-wave detectors will observe thousands of coalescing neutron star...
Second-generation interferometric gravitational-wave detectors, such as Advanced LIGO and Advanced V...
Understanding the properties of transient gravitational waves (GWs) and their sources is of broad in...
The coalescence of compact binaries containing neutron stars or black holes is one of the most promi...
International audienceGravitational waves provide a unique tool for observational astronomy. While t...
ABSTRACT Gravitational waves provide a unique tool for observational astronomy. Whi...
Gravitational waves provide a unique tool for observational astronomy. While the first LIGO–Virgo ca...
Gravitational waves provide a unique tool for observational astronomy. While the first LIGO–Virgo ca...
Bayesian parameter estimation is fast becoming the language of gravitational-wave astronomy. It is t...
A major challenge in gravitational-wave astrophysics is the interpretation of observations, which re...
We introduce new modules in the open-source PyCBC gravitational- wave astronomy toolkit that impleme...
The Advanced LIGO and Advanced Virgo gravitational-wave (GW) detectors will begin operation in the c...
The Advanced LIGO and Advanced Virgo gravitational wave (GW) detectors will begin operation in the c...
Detecting gravitational waves is just the start of the story; to understand their nature and the sys...
Third generation (3G) gravitational-wave detectors will observe thousands of coalescing neutron star...
Second-generation interferometric gravitational-wave detectors, such as Advanced LIGO and Advanced V...
Understanding the properties of transient gravitational waves (GWs) and their sources is of broad in...
The coalescence of compact binaries containing neutron stars or black holes is one of the most promi...