The mergers of double neutron star (NS–NS) and black hole (BH)–NS binaries are
promising gravitational wave (GW) sources for Advanced LIGO and future GW detectors. The …

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 …

On 17 August 2017, the Laser Interferometer Gravitational-Wave Observatory (LIGO) and the
Virgo interferometer detected gravitational waves (GWs) emanating from a binary neutron …

Abstract We present the Dark Energy Camera (DECam) discovery of the optical counterpart
of the first binary neutron star merger detected through gravitational-wave emission …

First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy
Survey Galaxies and the LIGO/Virgo Binary–Black-hole Merger GW170814 — Andrews …

We report Chandra observations of GW170817, the first neutron star–neutron star merger
discovered by the joint LIGO-Virgo Collaboration, and the first direct detection of …

We present a measurement of the Hubble constant H 0 using the gravitational wave (GW)
event GW190814, which resulted from the coalescence of a 23 M⊙ black hole with a 2.6 …

This Supplement provides supporting material for Abbott et al.(2016a). We briefly summarize
past electromagnetic (EM) follow-up efforts as well as the organization and policy of the …

Abstract Massive Primordial Black Holes (MPBH) can be formed after inflation due to broad
peaks in the primordial curvature power spectrum that collapse gravitationally during the …

Ejected material from neutron star mergers gives rise to electromagnetic emission powered
by radioactive decays of r-process nuclei, the so-called kilonova or macronova. While …