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 …

Significant progress has been made in recent years on the development of gravitational-
wave detectors. Sources such as coalescing compact binary systems, neutron stars in low …

A central challenge in gravitational wave astronomy is identifying weak signals in the
presence of non-stationary and non-Gaussian noise. The separation of gravitational wave …

The final inspiral of double neutron star and neutron-star–black-hole binaries are likely to be
detected by advanced networks of ground-based gravitational wave (GW) interferometers …

Abstract The LIGO Open Science Center (LOSC) fulfills LIGO's commitment to release,
archive, and serve LIGO data in a broadly accessible way to the scientific community and to …

This paper develops a general framework for studying the effectiveness of networks of
interferometric gravitational wave detectors and then uses it to show that enlarging the …

The Omicron software is a tool developed to perform a multi-resolution time–frequency
analysis of data from gravitational-wave detectors: the LIGO, Virgo, and KAGRA detectors …

We performed a detailed analysis of the detectability of a wide range of gravitational waves
derived from core-collapse supernova simulations using gravitational-wave detector noise …

The next galactic core-collapse supernova (CCSN) has already exploded, and its
electromagnetic (EM) waves, neutrinos, and gravitational waves (GWs) may arrive at any …

Gravitational wave science should transform in this decade from a study of what has not
been seen to a full-fledged field of astronomy in which detected signals reveal the nature of …