Gravitational waves provide a unique tool for observational astronomy. While the first LIGO–Virgo catalogue of gravitational-wave transients (GWTC-1) contains eleven 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 that it accurately...
The Advanced LIGO and Advanced Virgo gravitational-wave (GW) detectors will begin operation in the c...
We describe the implementation of a search for gravitational waves from compact binary coalescences ...
The Advanced LIGO and Advanced Virgo gravitational wave (GW) detectors will begin operation in the c...
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...
Gravitational waves provide a unique tool for observational astronomy. While the first LIGO–Virgo ca...
ABSTRACT Gravitational waves provide a unique tool for observational astronomy. Whi...
A major challenge in gravitational-wave astrophysics is the interpretation of observations, which re...
Bayesian parameter estimation is fast becoming the language of gravitational-wave astronomy. It is t...
We introduce new modules in the open-source PyCBC gravitational- wave astronomy toolkit that impleme...
The recently published GWTC-1 (Abbott B P et al (LIGO Scientific Collaboration and Virgo Collaborati...
The Nobel prize winning discovery of gravitational waves from a binary black hole merger GW150914 op...
The coalescence of compact binaries containing neutron stars or black holes is one of the most promi...
Coalescing compact binaries emitting gravitational wave (GW) signals, as recently detected by the A...
Advanced ground based laser interferometer gravitational wave detectors are due to come online in la...
The Advanced LIGO and Advanced Virgo gravitational-wave (GW) detectors will begin operation in the c...
We describe the implementation of a search for gravitational waves from compact binary coalescences ...
The Advanced LIGO and Advanced Virgo gravitational wave (GW) detectors will begin operation in the c...
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...
Gravitational waves provide a unique tool for observational astronomy. While the first LIGO–Virgo ca...
ABSTRACT Gravitational waves provide a unique tool for observational astronomy. Whi...
A major challenge in gravitational-wave astrophysics is the interpretation of observations, which re...
Bayesian parameter estimation is fast becoming the language of gravitational-wave astronomy. It is t...
We introduce new modules in the open-source PyCBC gravitational- wave astronomy toolkit that impleme...
The recently published GWTC-1 (Abbott B P et al (LIGO Scientific Collaboration and Virgo Collaborati...
The Nobel prize winning discovery of gravitational waves from a binary black hole merger GW150914 op...
The coalescence of compact binaries containing neutron stars or black holes is one of the most promi...
Coalescing compact binaries emitting gravitational wave (GW) signals, as recently detected by the A...
Advanced ground based laser interferometer gravitational wave detectors are due to come online in la...
The Advanced LIGO and Advanced Virgo gravitational-wave (GW) detectors will begin operation in the c...
We describe the implementation of a search for gravitational waves from compact binary coalescences ...
The Advanced LIGO and Advanced Virgo gravitational wave (GW) detectors will begin operation in the c...