Only numerical relativity simulations can capture the full complexities of binary black hole
mergers. These simulations, however, are prohibitively expensive for direct data analysis …

We introduce GWFAST, a novel Fisher-matrix code for gravitational-wave studies, tuned
toward third-generation gravitational-wave detectors such as Einstein Telescope (ET) and …

We study gravitational waves (GWs) induced by non-Gaussian curvature perturbations. We
calculate the density parameter per logarithmic frequency interval, Ω GW (k), given that the …

The first observational run of the Advanced LIGO detectors, from September 12, 2015 to
January 19, 2016, saw the first detections of gravitational waves from binary black hole …

Following a major upgrade, the two advanced detectors of the Laser Interferometer
Gravitational-wave Observatory (LIGO) held their first observation run between September …

Despite their long history and astrophysical importance, some of the key properties of
neutron stars are still uncertain. The extreme conditions encountered in their interiors …

Gravitational waves (GWs) from compact binary coalescences allow for the direct
measurement of the luminosity distance to their source. This makes them standard-distance …

We present the second Open Gravitational-wave Catalog (2-OGC) of compact-binary
coalescences, obtained from the complete set of public data from Advanced LIGO's first and …

The LIGO detection of GW150914 provides an unprecedented opportunity to study the two-
body motion of a compact-object binary in the large-velocity, highly nonlinear regime, and to …

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