Living Reviews in Relativity, 2018 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 information to the astronomy community to facilitate planning for multi-messenger ...
K g Arun, R Birney, M W Coughlin
exaly +3 more sources
Research on Interferometric Tilt Sensor for Vibration Isolation Platform [PDF]
SensorsLow-frequency seismic vibrations extremely limit the performance of ground simulation facilities for space-borne gravitational wave detections, which need to be substantially suppressed. Active vibration systems are thus required.
Weigang Bai +4 more
doaj +2 more sources
Living Reviews in Relativity, 2016 We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger ...
K g Arun, R Birney, M W Coughlin
exaly +3 more sources
Modeling and Simulation of Inter-Satellite Laser Communication for Space-Based Gravitational Wave Detection [PDF]
SensorsSpace-based gravitational wave detection uses an equilateral triangular satellite constellation with inter-satellite laser heterodyne interferometry to measure displacement variations caused by gravitational waves.
Haoqian Liang +3 more
doaj +2 more sources
Defining eccentricity for gravitational wave astronomy [PDF]
Physical Review D, 2023 Eccentric compact binary mergers are significant scientific targets for current and future gravitational wave observatories. To detect and analyze eccentric signals, there is an increasing effort to develop waveform models, numerical relativity ...
Md Arif Shaikh +4 more
semanticscholar +1 more source
Quiescent and Active Galactic Nuclei as Factories of Merging Compact Objects in the Era of Gravitational Wave Astronomy [PDF]
Universe, 2023 Galactic nuclei harbouring a central supermassive black hole (SMBH), possibly surrounded by a dense nuclear cluster (NC), represent extreme environments that house a complex interplay of many physical processes that uniquely affect stellar formation ...
M. A. Sedda, S. Naoz, B. Kocsis
semanticscholar +1 more source
When models fail: An introduction to posterior predictive checks and model misspecification in gravitational-wave astronomy [PDF]
Publications Astronomical Society of Australia, 2022 Bayesian inference is a powerful tool in gravitational-wave astronomy. It enables us to deduce the properties of merging compact-object binaries and to determine how these mergers are distributed as a population according to mass, spin, and redshift.
I. Romero-Shaw, E. Thrane, P. Lasky
semanticscholar +1 more source
Nanohertz gravitational wave astronomy during SKA era: An InPTA perspective [PDF]
Journal of astrophysics and astronomy, 2022 Decades long monitoring of millisecond pulsars, which exhibit highly stable rotational periods in pulsar timing array experiments is on the threshold of discovering nanohertz stochastic gravitational wave background.
B. C. Joshi +65 more
semanticscholar +1 more source
Do unequal-mass binary black hole systems have larger $\chi_\text{eff}$? Probing correlations with copulas in gravitational-wave astronomy [PDF]
, 2022 The formation history of binary black hole systems is imprinted on the distribution of their masses, spins, and eccentricity. While much has been learned studying these parameters in turn , recent studies have explored the joint distribution of binary ...
C. Adamcewicz, E. Thrane
semanticscholar +1 more source
Gaussian processes for Glitch-robust Gravitational-wave astronomy [PDF]
Monthly notices of the Royal Astronomical Society, 2022 Interferometric gravitational-wave observatories have opened a new era in astronomy. The rich data produced by an international network enables detailed analysis of the curved space-time around black holes.
G. Ashton
semanticscholar +1 more source