Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA
BP Abbott, R Abbott, TD Abbott, S Abraham… - Living reviews in …, 2020 - Springer
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 …
LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next several years …
Rates of compact object coalescences
Gravitational-wave detections are enabling measurements of the rate of coalescences of
binaries composed of two compact objects—neutron stars and/or black holes. The …
binaries composed of two compact objects—neutron stars and/or black holes. The …
Compact radio emission indicates a structured jet was produced by a binary neutron star merger
The binary neutron star merger event GW170817 was detected through both
electromagnetic radiation and gravitational waves. Its afterglow emission may have been …
electromagnetic radiation and gravitational waves. Its afterglow emission may have been …
First multimessenger observations of a neutron star merger
R Margutti, R Chornock - Annual Review of Astronomy and …, 2021 - annualreviews.org
We describe the first observations of the same celestial object with gravitational waves and
light.▪ GW170817 was the first detection of a neutron star merger with gravitational waves.▪ …
light.▪ GW170817 was the first detection of a neutron star merger with gravitational waves.▪ …
The giant radio array for neutrino detection (GRAND): science and design
Abstract The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale
observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 10 8 GeV …
observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 10 8 GeV …
The optical afterglow of GW170817 at one year post-merger
We present observations of the optical afterglow of GRB 170817A, made by the Hubble
Space Telescope, between 2018 February and August, up to one year after the neutron star …
Space Telescope, between 2018 February and August, up to one year after the neutron star …
An assessment of the association between a fast radio burst and binary neutron star merger
Fast radio bursts (FRBs) are bright millisecond-duration radio bursts at cosmological
distances. While young magnetars are the leading source candidate, recent observations …
distances. While young magnetars are the leading source candidate, recent observations …
A peculiarly short-duration gamma-ray burst from massive star core collapse
Gamma-ray bursts (GRBs) have been phenomenologically classified into long and short
populations based on the observed bimodal distribution of duration. Multi-wavelength and …
populations based on the observed bimodal distribution of duration. Multi-wavelength and …
Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA
Kagra Collaboration… - Living Reviews in …, 2018 - research.monash.edu
We present possible observing scenarios for the Advanced LIGO, Advanced Virgo and
KAGRA gravitational-wave detectors over the next decade, with the intention of providing …
KAGRA gravitational-wave detectors over the next decade, with the intention of providing …
Constraints on the maximum mass of neutron stars with a quark core from GW170817 and NICER PSR J0030+ 0451 data
We perform a Bayesian analysis of the maximum mass M TOV of neutron stars with a quark
core, incorporating the observational data from tidal deformability of the GW170817 binary …
core, incorporating the observational data from tidal deformability of the GW170817 binary …