LIGO detector characterization in the second and third observing runs
The characterization of the Advanced LIGO detectors in the second and third observing runs
has increased the sensitivity of the instruments, allowing for a higher number of detectable …
has increased the sensitivity of the instruments, allowing for a higher number of detectable …
Neutron star-black hole mergers in next generation gravitational-wave observatories
Observations by the current generation of gravitational-wave detectors have been pivotal in
expanding our understanding of the universe. Although tens of exciting compact binary …
expanding our understanding of the universe. Although tens of exciting compact binary …
Listening to the universe with next generation ground-based gravitational-wave detectors
S Borhanian, BS Sathyaprakash - Physical Review D, 2024 - APS
In this study, we use simple performance metrics to assess the science capabilities of future
ground-based gravitational-wave detector networks composed of A+ or Voyager upgrades …
ground-based gravitational-wave detector networks composed of A+ or Voyager upgrades …
Rapid premerger localization of binary neutron stars in third-generation gravitational-wave detectors
Premerger localization of binary neutron stars (BNSs) is one of the most important scientific
goals for the third-generation (3G) gravitational-wave detectors. It will enable the …
goals for the third-generation (3G) gravitational-wave detectors. It will enable the …
Kilonova Emission from Black Hole–Neutron Star Mergers. II. Luminosity Function and Implications for Target-of-opportunity Observations of Gravitational-wave …
We present detailed simulations of the kilonova and gamma-ray burst (GRB) afterglow and
kilonova luminosity function from black hole–neutron star (BH–NS) mergers, and discuss the …
kilonova luminosity function from black hole–neutron star (BH–NS) mergers, and discuss the …
Gravitational-wave merger forecasting: Scenarios for the early detection and localization of compact-binary mergers with ground-based observatories
AH Nitz, M Schäfer, T Dal Canton - The Astrophysical Journal …, 2020 - iopscience.iop.org
We present the prospects for the early (pre-merger) detection and localization of compact-
binary coalescences using gravitational waves over the next 10 yr. Early warning can …
binary coalescences using gravitational waves over the next 10 yr. Early warning can …
Pre-merger localization of compact-binary mergers with third-generation observatories
AH Nitz, T Dal Canton - The Astrophysical Journal Letters, 2021 - iopscience.iop.org
We present the prospects for the pre-merger detection and localization of binary neutron star
mergers with third-generation gravitational-wave (GW) observatories. We consider a wide …
mergers with third-generation gravitational-wave (GW) observatories. We consider a wide …
Kilonovae and Optical Afterglows from Binary Neutron Star Mergers. II. Optimal Search Strategy for Serendipitous Observations and Target-of-opportunity …
In the second work of this series, we explore the optimal search strategy for serendipitous
and gravitational-wave-triggered target-of-opportunity (ToO) observations of kilonovae and …
and gravitational-wave-triggered target-of-opportunity (ToO) observations of kilonovae and …
Gear Up for the Action Replay: Leveraging Lensing for Enhanced Gravitational-wave Early Warning
Premerger gravitational-wave (GW) sky localization of binary neutron star (BNS) and
neutron star–black hole (NSBH) coalescence events would enable telescopes to capture …
neutron star–black hole (NSBH) coalescence events would enable telescopes to capture …
Eccentricity enables the earliest warning and localization of gravitational waves with ground-based detectors
The early and precise localization of gravitational waves (GWs) is pivotal in detecting their
electromagnetic (EM) counterparts, especially for binary neutron stars (BNS) and neutron …
electromagnetic (EM) counterparts, especially for binary neutron stars (BNS) and neutron …