Advanced Virgo: a 2nd generation interferometric gravitational wave detector

Abstract

Advanced Virgo is the project to upgrade the Virgo interferometric detector of gravitational waves, with the aim of increasing the number of observable galaxies (and thus the detection rate) by three orders of magnitude. The project is now in an advanced construction phase and the assembly and integration will be completed by the end of 2015. Advanced Virgo will be part of a network with the two Advanced LIGO detectors in the US and GEO HF in Germany, with the goal of contributing to the early detections of gravitational waves and to opening a new observation window on the universe. In this paper we describe the main features of the Advanced Virgo detector and outline the status of the construction.

Submitted to Classical and Quantum Gravity. 55 pages, 29 figures

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• Constraints on ultralight scalar bosons within black hole spin measurements from LIGO-Virgo's GWTC-2
• Parameter estimation for heavy binary-black holes with networks of second-generation gravitational-wave detectors
• Dark stars: gravitational and electromagnetic observables
• A Multipolar Effective One Body Model for Non-Spinning Black Hole Binaries
• Testing the general theory of relativity using gravitational wave propagation from dark standard sirens
• A Refined Einstein-Gauss-Bonnet Inflationary Theoretical Framework
• Radio Counterparts of Compact Binary Mergers detectable in Gravitational Waves: A Simulation for an Optimized Survey
• Detecting Stellar Lensing of Gravitational Waves with Ground-Based Observatories
• Gravitational-wave physics with Cosmic Explorer: limits to low-frequency sensitivity
• Review of the Advanced LIGO gravitational wave observatories leading to observing run four
• Gravitational-Wave Asteroseismology with Fundamental Modes from Compact Binary Inspirals
• The fifth-order post-Newtonian Hamiltonian dynamics of two-body systems from an effective field theory approach: potential contributions
• A light in the dark: searching for electromagnetic counterparts to black hole-black hole mergers in LIGO/Virgo O3 with the Zwicky Transient Facility
• Classical gravitational spinning-spinless scattering at $\mathcal{O}(G^2{S}^{\infty })$
• Measuring the spectrum of primordial gravitational waves with CMB, PTA and Laser Interferometers
• The Most Massive Binary Black Hole Detections and the Identification of Population Outliers
• A First Targeted Search for Gravitational-Wave Bursts from Core-Collapse Supernovae in Data of First-Generation Laser Interferometer Detectors
• An aligned-spin neutron-star--black-hole waveform model based on the effective-one-body approach and numerical-relativity simulations
• A Detailed Examination of Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of ${}^{208}$Pb with Minimal Modeling Assumptions
• A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries
• Search for intermediate mass black hole binaries in the third observing run of Advanced LIGO and Advanced Virgo
• Cover Your Basis: Comprehensive Data-Driven Characterization of the Binary Black Hole Population
• A complete cosmological scenario from $f(R,T^{\phi })$ gravity theory
• Mechanical loss in state-of-the-art amorphous optical coatings
• The unpolarized macronova associated with the gravitational wave event GW170817
• A data science platform to enable time-domain astronomy
• Observing the post-merger signal of GW170817-like events with improved gravitational-wave detectors
• Orbital Evolution of Binaries in Circumbinary Disks
• Inferring the properties of a population of compact binaries in presence of selection effects
• Axion Dark Matter Search with Interferometric Gravitational Wave Detectors
• Gravitational Wave and CMB Probes of Axion Kination
• Merger rate of black hole binaries from globular clusters: theoretical error bars and comparison to gravitational wave data from GWTC-2
• Hunt for Light Primordial Black Hole Dark Matter with Ultra-High-Frequency Gravitational Waves
• Terrestrial Gravity Fluctuations
• Deep-Learning continuous gravitational waves
• Search for ultralight bosons in Cygnus X-1 with Advanced LIGO
• Polarization-based Tests of Gravity with the Stochastic Gravitational-Wave Background
• Enhancing the bandwidth of gravitational-wave detectors with unstable optomechanical filters
• Gwbench: a novel Fisher information package for gravitational-wave benchmarking
• Studying strong phase transitions in neutron stars with gravitational waves
• Probing multiple populations of compact binaries with third-generation gravitational-wave detectors
• Evidence for a minimum ellipticity in millisecond pulsars
• Astrophysics and cosmology with a decihertz gravitational-wave detector: TianGO
• The curious case of GW200129: interplay between spin-precession inference and data-quality issues
• Anisotropies in the astrophysical gravitational-wave background: Predictions for the detection of compact binaries by LIGO and Virgo
• Fast-transient Searches in Real Time with ZTFReST: Identification of Three Optically-discovered Gamma-ray Burst Afterglows and New Constraints on the Kilonova Rate
• IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes
• THESEUS: a key space mission concept for Multi-Messenger Astrophysics
• The final twist: A model of gravitational waves from precessing black-hole binaries through merger and ringdown
• Frequency-Dependent Responses in 3rd Generation Gravitational-Wave Detectors
• Searching for the full symphony of black hole binary mergers
• Dark Sirens to Resolve the Hubble-Lemaître Tension
• Constraints on Einstein-dilaton-Gauss-Bonnet gravity from Black Hole-Neutron Star Gravitational Wave Events
• Observing intermediate-mass black holes and the upper--stellar-mass gap with LIGO and Virgo
• Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes II. Spins and Incoming Objects
• Identifying strong gravitational-wave lensing during the second observing run of Advanced LIGO and Advanced Virgo
• Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data
• Tests of General Relativity with Gravitational-Wave Observations using a Flexible--Theory-Independent Method
• Constraints on dark photon dark matter using data from LIGO's and Virgo's third observing run
• Noise Reduction in Gravitational-wave Data via Deep Learning
• Inferring the core-collapse supernova explosion mechanism with gravitational waves
• Shadow images of Kerr-like wormholes
• Can we distinguish astrophysical from primordial black holes via the stochastic gravitational wave background?
• A Fourier Domain Waveform for Non-Spinning Binaries with Arbitrary Eccentricity
• Narrow-band search for gravitational waves from known pulsars using the second LIGO observing run
• A comparison between short GRB afterglows and AT2017gfo: shedding light on kilonovae properties
• Subtracting compact binary foreground sources to reveal primordial gravitational-wave backgrounds
• Current observations are insufficient to confidently associate the binary black hole merger GW190521 with AGN J124942.3+344929
• Impact of inter-correlated initial binary parameters on double black hole and neutron star mergers
• The Influence of Neutrinos on r-Process Nucleosynthesis in the Ejecta of Black Hole-Neutron Star Mergers
• Forecasts for detecting the gravitational-wave memory effect with Advanced LIGO and Virgo
• MHz Gravitational Wave Constraints with Decameter Michelson Interferometers
• All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run
• Enhancing the SEOBNRv5 effective-one-body waveform model with second-order gravitational self-force fluxes
• Supernova Model Discrimination with Hyper-Kamiokande
• Picky Partners: The Pairing of Component Masses in Binary Black Hole Mergers
• Intermediate mass black holes from stellar mergers in young star clusters
• Towards mitigation of apparent tension between nuclear physics and astrophysical observations by improved modeling of neutron star matter
• Bilby-MCMC: An MCMC sampler for gravitational-wave inference
• PhenomXO4a: a phenomenological gravitational-wave model for precessing black-hole binaries with higher multipoles and asymmetries
• When are LIGO/Virgo's Big Black-Hole Mergers?
• Updated constraints on amplitude and tilt of the tensor primordial spectrum
• Distinguishing the nature of comparable-mass neutron star binary systems with multimessenger observations: GW170817 case study
• Parameterized tests of the strong-field dynamics of general relativity using gravitational wave signals from coalescing binary black holes: Fast likelihood calculations and sensitivity of the method
• Stochastic gravitational-wave background as a tool to investigate multi-channel astrophysical and primordial black-hole mergers
• Search for strongly lensed counterpart images of binary black hole mergers in the first two LIGO observing runs
• Waveform systematics in the gravitational-wave inference of tidal parameters and equation of state from binary neutron star signals
• Binary black holes population and cosmology in new lights: Signature of PISN mass and formation channel in GWTC-3
• Fast and Accurate Sensitivity Estimation for Continuous-Gravitational-Wave Searches
• Quasinormal-mode filters: a new approach to analyze the gravitational-wave ringdown of binary black-hole mergers
• Black Hole Formation in the Lower Mass Gap through Mergers and Accretion in AGN Disks
• A detailed analysis of GW190521 with phenomenological waveform models
• Formation channels of single and binary stellar-mass black holes
• Hierarchical test of general relativity with gravitational waves
• On the origin of GW190425
• Discovering features in gravitational-wave data through detector characterization, citizen science and machine learning
• Noise spectral estimation methods and their impact on gravitational wave measurement of compact binary mergers
• Black-hole ringdown as a probe of higher-curvature gravity theories
• Gravitational-wave cutoff frequencies of tidally disruptive neutron star-black hole binary mergers
• Beyond the detector horizon: Forecasting gravitational-wave strong lensing
• Impact of PREX-II and combined Radio/NICER/XMM-Newton's mass-radius measurement of PSRJ0740+6620 on the dense matter equation of state
• Modeling and searching for a stochastic gravitational-wave background from ultralight vector bosons
• Frequency-domain gravitational waveform models for inspiraling binary neutron stars
• Search for Eccentric Binary Neutron Star Mergers in the first and second observing runs of Advanced LIGO
• Comparing two models for measuring the neutron star equation of state from gravitational-wave signals
• The Detected Stochastic Gravitational Waves and Subsolar-Mass Primordial Black Holes
• Template-based Gravitational-Wave Echoes Search Using Bayesian Model Selection
• The Mass Distribution of Neutron Stars in Gravitational-wave Binaries
• Applications and Techniques for Fast Machine Learning in Science
• Evidence for an intermediate-mass black hole from a gravitationally lensed gamma-ray burst
• Detection and Classification of Supernova Gravitational Waves Signals: A Deep Learning Approach
• The first six months of the Advanced LIGO's and Advanced Virgo's third observing run with GRANDMA
• Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network
• Testing the nature of gravitational-wave polarizations using strongly lensed signals
• Gravitational wave forest from string axiverse
• Constraints on the moment of inertia of PSR J0737-3039A from GW170817
• The Hitchhiker's guide to the galaxy catalog approach for gravitational wave cosmology
• Spin effects on neutron star fundamental-mode dynamical tides: phenomenology and comparison to numerical simulations
• High Eccentricities and High Masses Characterize Gravitational-wave Captures in Galactic Nuclei as Seen by Earth-based Detectors
• Inferring the population properties of binary neutron stars with gravitational-wave measurements of spin
• Advanced quantum techniques for future gravitational-wave detectors
• A hybrid post-Newtonian -- effective-one-body scheme for spin-precessing compact-binary waveforms
• Subtracting glitches from gravitational-wave detector data during the third observing run
• The binary black hole spin distribution likely broadens with redshift
• Searches for continuous gravitational waves from neutron stars: A twenty-year retrospective
• Searches for Gravitational Waves from Known Pulsars at Two Harmonics in the Second and Third LIGO-Virgo Observing Runs
• Narrowband searches for continuous and long-duration transient gravitational waves from known pulsars in the LIGO-Virgo third observing run
• Towards Robust Gravitational Wave Detection with Pulsar Timing Arrays
• Accelerating parameter estimation of gravitational waves from compact binary coalescence using adaptive frequency resolutions
• Measurement and subtraction of Schumann resonances at gravitational-wave interferometers
• Binary Black Hole Mergers from LIGO/Virgo O1 and O2: Population Inference Combining Confident and Marginal Events
• Inferring prompt black-hole formation in neutron star mergers from gravitational-wave data
• Jumping the gap: searching for LIGO's biggest black holes
• Optimizing searches for electromagnetic counterparts of gravitational wave triggers
• Dynamical ejecta from precessing neutron star-black hole mergers with a hot, nuclear-theory based equation of state
• Directional limits on persistent gravitational waves using data from Advanced LIGO's first two observing runs
• Discriminating between Neutron Stars and Black Holes with Imperfect Knowledge of the Maximum Neutron Star Mass
• Strong-field scattering of two black holes: Numerical Relativity meets Post-Minkowskian gravity
• Exploring Features in the Binary Black Hole Population
• Apples and Oranges: Comparing black holes in X-ray binaries and gravitational-wave sources
• Third post-Newtonian gravitational waveforms for compact binary systems in general orbits: Instantaneous terms
• Parameter estimation on gravitational waves from neutron-star binaries with spinning components
• Effective one-body model for extreme-mass-ratio spinning binaries on eccentric equatorial orbits: testing radiation reaction and waveform
• Overview of Advanced LIGO Adaptive Optics
• A first survey of spinning eccentric black hole mergers: Numerical relativity simulations, hybrid waveforms, and parameter estimation
• Modeling the postmerger gravitational wave signal and extracting binary properties from future binary neutron star detections
• Light-curve models of black hole - neutron star mergers: steps towards a multi-messenger parameter estimation
• Counting Black Holes: The Cosmic Stellar Remnant Population and Implications for LIGO
• Equation-of-state insensitive relations after GW170817
• Search for light scalar Dark Matter candidate with AURIGA detector
• Stochastic Gravitational Wave Background from Global Cosmic Strings
• Properties of the stochastic astrophysical gravitational wave background: astrophysical sources dependencies
• All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems
• How effective is machine learning to detect long transient gravitational waves from neutron stars in a real search?
• Does Matter Matter? Using the mass distribution to distinguish neutron stars and black holes
• Supercooling in Radiative Symmetry Breaking: Theory Extensions, Gravitational Wave Detection and Primordial Black Holes
• Multi-messenger observations of binary neutron star mergers in the O4 run
• Search for continuous gravitational wave emission from the Milky Way center in O3 LIGO--Virgo data
• Modelling Neutron Star-Black Hole Binaries: Future Pulsar Surveys and Gravitational Wave Detectors
• Time-dependence of the astrophysical stochastic gravitational wave background
• Biases in parameter estimation from overlapping gravitational-wave signals in the third generation detector era
• Gravitational waves and kicks from the merger of unequal mass, highly compact boson stars
• Search for subsolar-mass binaries in the first half of Advanced LIGO and Virgo's third observing run
• Neutron Star Mergers and How to Study Them
• Importance of mirror modes in binary black hole ringdown waveform
• A Parameter-Free Tour of the Binary Black Hole Population
• All-sky Search for Continuous Gravitational Waves from Isolated Neutron Stars in the Early O3 LIGO Data
• Prospects for detecting gravitational waves at 5 Hz with ground-based detectors
• Measurement Accuracy of Inspiraling Eccentric Neutron Star and Black Hole Binaries Using Gravitational Waves
• Defining eccentricity for gravitational wave astronomy
• Intermediate mass-ratio black hole binaries: Applicability of small mass-ratio perturbation theory
• Preparing the next gravitational million-body simulations: Evolution of single and binary stars in Nbody6++GPU, MOCCA and McLuster
• Updated Constraints and Forecasts on Primordial Tensor Modes
• Validating gravitational-wave detections: The Advanced LIGO hardware injection system
• An approach to computing spectral shifts for black holes beyond Kerr
• A morphology-independent data analysis method for detecting and characterizing gravitational wave echoes
• Importance of transient resonances in extreme-mass-ratio inspirals
• Implications for First-Order Cosmological Phase Transitions from the Third LIGO-Virgo Observing Run
• Gravitational-Wave Localization Alone Probes AGN Origin of Stellar-Mass Black Hole Mergers
• Low mechanical loss TiO${}_2$:GeO${}_2$ coatings for reduced thermal noise in Gravitational Wave Interferometers
• The ANTARES Astronomical Time-Domain Event Broker
• Sub-radian-accuracy gravitational waves from coalescing binary neutron stars II: Systematic study on the equation of state, binary mass, and mass ratio
• Gravitational spin-orbit coupling through third-subleading post-Newtonian order: from first-order self-force to arbitrary mass ratios
• POEMMA's Target of Opportunity Sensitivity to Cosmic Neutrino Transient Sources
• Spectral separation of the stochastic gravitational-wave background for LISA: observing both cosmological and astrophysical backgrounds
• Constraining gravitational wave amplitude birefringence and Chern-Simons gravity with GWTC-2
• A morphology-independent search for gravitational wave echoes in data from the first and second observing runs of Advanced LIGO and Advanced Virgo
• On the growth of massive scalar hair around a Schwarzschild black hole
• Pan-STARRS and PESSTO search for an optical counterpart to the LIGO gravitational wave source GW150914
• Search for gravitational waves from Scorpius X-1 in the second Advanced LIGO observing run with an improved hidden Markov model
• Accuracy of Estimating Highly Eccentric Binary Black Hole Parameters with Gravitational-Wave Detections
• Extracting the Gravitational Recoil from Black Hole Merger Signals
• MLGWSC-1: The first Machine Learning Gravitational-Wave Search Mock Data Challenge
• Outflow Bubbles from Compact Binary Mergers Embedded in Active Galactic Nuclei: Cavity Formation and the Impact on Electromagnetic Counterparts
• Broad search for gravitational waves from subsolar-mass binaries through LIGO and Virgo's third observing run
• Measuring the neutron star equation of state with gravitational waves: the first forty binary neutron star mergers
• A fast and precise methodology to search for and analyse strongly lensed gravitational-wave events
• Applying deep neural networks to the detection and space parameter estimation of compact binary coalescence with a network of gravitational wave detectors
• Gravitational-wave memory: waveforms and phenomenology
• Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds
• GWFish: A simulation software to evaluate parameter-estimation capabilities of gravitational-wave detector networks
• No evidence that the majority of black holes in binaries have zero spin
• The fifth-order post-Newtonian Hamiltonian dynamics of two-body systems from an effective field theory approach
• Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions
• Constraining black hole mimickers with gravitational wave observations
• Search for gravitational waves from the coalescence of sub-solar mass binaries in the first half of Advanced LIGO and Virgo's third observing run
• GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
• Black hole kicks as new gravitational wave observables
• Standard Siren Speeds: Improving velocities in gravitational-wave measurements of $H_0$
• Constraints on Kerr-Newman black holes from merger-ringdown gravitational-wave observations
• Search methods for continuous gravitational-wave signals from unknown sources in the advanced-detector era
• Imprint of a scalar era on the primordial spectrum of gravitational waves
• The Impact of Peculiar Velocities on the Estimation of the Hubble Constant from Gravitational Wave Standard Sirens
• Searches After Gravitational-waves Using ARizona Observatories (SAGUARO): System Overview and First Results from Advanced LIGO/Virgo's Third Observing Run
• Polarization test of gravitational waves from compact binary coalescences
• GW190814: On the properties of the secondary component of the binary
• Primordial Gravitational Wave Signals in Modified Cosmologies
• Parameter estimation for black hole echo signals and their statistical significance
• An alternative interpretation of GW190412 as a binary black hole merger with a rapidly spinning secondary
• Detection and localization of single-source gravitational waves with pulsar timing arrays
• Estimating the angular power spectrum of the gravitational-wave background in the presence of shot noise
• Incompleteness Matters Not: Inference of $H_0$ from BBH-galaxy cross-correlations
• Probing planetary-mass primordial black holes with continuous gravitational waves
• Joint gravitational wave -- gamma-ray burst detection rates in the aftermath of GW170817
• Hereditary Terms at Next-To-Leading Order in Two-Body Gravitational Dynamics
• Impact of Dynamical Tides on the Reconstruction of the Neutron Star Equation of State
• Parameter Estimation with a spinning multi-mode waveform model: IMRPhenomHM
• Probing circular polarization in stochastic gravitational wave background with pulsar timing arrays
• Foreground cleaning and template-free stochastic background extraction for LISA
• Primordial backgrounds of relic gravitons
• Ramsey-Bordé matter-wave interferometry for laser frequency stabilization at $10^{-16}$ frequency instability and below
• Characterising Transient Noise in the LIGO Detectors
• Observability of lensing of gravitational waves from massive black hole binaries with LISA
• On the dynamical bar-mode instability in spinning bosonic stars
• Gravitational waveforms from SpEC simulations : neutron star-neutron star and low-mass black hole-neutron star binaries
• Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors
• A Mock Data and Science Challenge for Detecting an Astrophysical Stochastic Gravitational-Wave Background with Advanced LIGO and Advanced Virgo
• Search for continuous gravitational waves from 20 accreting millisecond X-ray pulsars in O3 LIGO data
• Parameter Estimation and Model Selection of Gravitational Wave Signals Contaminated by Transient Detector Noise Glitches
• Tracking black hole kicks from gravitational wave observations
• Enhancing modified gravity detection from gravitational-wave observations using the Parametrized ringdown spin expansion coefficients formalism
• GW190412 as a Third-Generation Black Hole Merger from a Super Star Cluster
• The astrophysical science case for a decihertz gravitational-wave detector
• Virgo Detector Characterization and Data Quality: results from the O3 run
• Rapid Parameter Estimation of Gravitational Waves from Binary Neutron Star Coalescence using Focused Reduced Order Quadrature
• Relevance of tidal effects and post-merger dynamics for binary neutron star parameter estimation
• Spin dependence of black hole ringdown nonlinearities
• Neutron stars versus black holes: probing the mass gap with LIGO/Virgo
• StarTrack predictions of the stochastic gravitational-wave background from compact binary mergers
• LIGO Detector Characterization in the first half of the fourth Observing run
• R&D around a photoneutralizer-based NBI system (Siphore) in view of a DEMO Tokamak steady state fusion reactor
• Towards inference of overlapping gravitational wave signals
• Gravitational-wave parameter estimation with gaps in LISA: a Bayesian data augmentation method
• Black hole mergers of AGN origin in LIGO/Virgo's O1-O3a observing periods
• Efficient Gravitational-wave Glitch Identification from Environmental Data Through Machine Learning
• A low-mass binary neutron star: long-term ejecta evolution and kilonovae with weak blue emission
• Modeling compact binary signals and instrumental glitches in gravitational wave data
• The Memory Remains (Undetected): Updates from the Second LIGO/Virgo Gravitational-Wave Transient Catalog
• Kilonova Detectability with Wide-Field Instruments
• Gravitational waves from Sco X-1: A comparison of search methods and prospects for detection with advanced detectors
• Effectual gravitational-wave template banks for coalescing compact binaries using a hybrid placement algorithm
• Dark photon superradiance: Electrodynamics and multimessenger signals
• First cryogenic test operation of underground km-scale gravitational-wave observatory KAGRA
• Data quality up to the third observing run of Advanced LIGO: Gravity Spy glitch classifications
• Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model
• Massively Parallel Simulations of Binary Black Hole Intermediate-Mass-Ratio Inspirals
• Towards the Design of Gravitational-Wave Detectors for Probing Neutron-Star Physics
• Modelling Double Neutron Stars: Radio and Gravitational Waves
• Calibration of Advanced Virgo and Reconstruction of the Gravitational Wave Signal h(t) during the Observing Run O2
• The stochastic gravitational-wave background in the absence of horizons
• You Can't Always Get What You Want: The Impact of Prior Assumptions on Interpreting GW190412
• High rate of gravitational waves mergers from flyby perturbations of wide black-hole triples in the field
• Tests of Gravitational-Wave Birefringence with the Open Gravitational-Wave Catalog
• The 6th Post-Newtonian Potential Terms at $O(G_N^4)$
• Bayesian statistical framework for identifying strongly lensed gravitational-wave signals
• The Advanced LIGO Input Optics
• Mass and rate of hierarchical black hole mergers in young, globular and nuclear star clusters
• State of the field: Binary black hole natal kicks and prospects for isolated field formation after GWTC-2
• Neutrino pair annihilation above merger remnants: implications of a long-lived massive neutron star
• Binary Neutron Stars with Arbitrary Spins in Numerical Relativity
• Searching for ultralight bosons within spin measurements of a population of binary black hole mergers
• Search for transient gravitational wave signals associated with magnetar bursts during Advanced LIGO's second observing run
• Probing the seesaw scale with gravitational waves
• Shot noise in the astrophysical gravitational-wave background
• Beating the standard sensitivity-bandwidth limit of cavity-enhanced interferometers with internal squeezed-light generation
• Waveform accuracy and systematic uncertainties in current gravitational wave observations
• Atomic source selection in space-borne gravitational wave detection
• Gravitational Waves from Fundamental Axion Dynamics
• The effect of $f(R,T)$ modified gravity on mass and radius of pulsar HerX1
• Searching for cosmological gravitational-wave backgrounds with third-generation detectors in the presence of an astrophysical foreground
• Can a black hole-neutron star merger explain GW170817, AT2017gfo, GRB170817A?
• Shock-powered radio precursors of neutron star mergers from accelerating relativistic binary winds
• Simultaneous estimation of astrophysical and cosmological stochastic gravitational-wave backgrounds with terrestrial detectors
• The final core collapse of pulsational pair instability supernovae
• Updated observing scenarios and multi-messenger implications for the International Gravitational-wave Network's O4 and O5
• Inference on gravitational waves from coalescences of stellar-mass compact objects and intermediate-mass black holes
• Subtraction of correlated noise in global networks of gravitational-wave interferometers
• Status and perspectives of Continuous Gravitational Wave searches
• Observable signature of merging stellar-mass black holes in active galactic nuclei
• Targeted large mass ratio numerical relativity surrogate waveform model for GW190814
• Kilonova Emission From Black Hole-Neutron Star Mergers. II. Luminosity Function and Implications for Target-of-opportunity Observations of Gravitational-wave Triggers and Blind Searches
• Inference of proto-neutron star properties from gravitational-wave data in core-collapse supernovae
• Testing Einstein's Weak Equivalence Principle With Gravitational Waves
• Modeling horizon absorption in spinning binary black holes using effective worldline theory
• Phase Transition Phenomenology with Nonparametric Representations of the Neutron Star Equation of State
• Order in the chaos: eccentric black hole binary mergers in triples formed via strong binary-binary scatterings
• Assessing the impact of transient orbital resonances
• A semi-coherent analysis method to search for continuous gravitational waves emitted by ultra-light boson clouds around spinning black holes
• Primordial gravitational waves and the H0-tension problem
• Testing the multipole structure of compact binaries using gravitational wave observations
• SuperRad: Modeling the black hole superradiance gravitational waveform
• Site-selection criteria for the Einstein Telescope
• Imposing multi-physics constraints at different densities on the Neutron Star Equation of State
• Improved ranking statistics of the GstLAL inspiral search for compact binary coalescences
• Generic searches for alternative gravitational wave polarizations with networks of interferometric detectors
• The SXS Collaboration's third catalog of binary black hole simulations
• Gravitational waves from first-order phase transitions: Ultra-supercooled transitions and the fate of relativistic shocks
• Tests of general relativity in the nonlinear regime: a parametrized plunge-merger-ringdown gravitational waveform model
• A new spin on LIGO-Virgo binary black holes
• Implications of the search for optical counterparts during the second part of the Advanced LIGO's and Advanced Virgo's third observing run: lessons learned for future follow-up observations
• The status of KAGRA underground cryogenic gravitational wave telescope
• The time delay distribution and formation metallicity of LIGO-Virgo's binary black holes
• When will we observe binary black holes precessing?
• Binary Neutron Star Merger Simulations with a Calibrated Turbulence Model
• Non-parametric inference of the population of compact binaries from gravitational wave observations using binned Gaussian processes
• Progress in the measurement and reduction of thermal noise in optical coatings for gravitational-wave detectors
• Black hole merger simulations in wave dark matter environments
• PERLE: Powerful Energy Recovery Linac for Experiments - Conceptual Design Report
• Waveform uncertainty quantification and interpretation for gravitational-wave astronomy
• Modeling dynamical scalarization with a resummed post-Newtonian expansion
• Capturing the electromagnetic counterparts of binary neutron star mergers through low latency gravitational wave triggers
• Quasinormal Modes of Black Holes with Non-Linear-Electrodynamic sources in Rastall Gravity
• Eigenvalue repulsions in the quasinormal spectra of the Kerr-Newman black hole
• Search for nonlinear memory from subsolar mass compact binary mergers
• The fates of massive stars: exploring uncertainties in stellar evolution with METISSE
• Improving gravitational-wave parameter estimation using Gaussian process regression
• Astrophysical constraints on compact objects in 4D Einstein-Gauss-Bonnet gravity
• The impact of the crust equation of state on the analysis of GW170817
• Horizons: Nuclear Astrophysics in the 2020s and Beyond
• Deep Learning Ensemble for Real-time Gravitational Wave Detection of Spinning Binary Black Hole Mergers
• Gravitational-wave astronomy with a physical calibration model
• Resolving The Peak Of The Black Hole Mass Spectrum
• Modelling the Ringdown from Precessing Black Hole Binaries
• GROWTH on S190426c. II. Real-Time Search for a Counterpart to the Probable Neutron Star-Black Hole Merger using an Automated Difference Imaging Pipeline for DECam
• Deep learning and Bayesian inference of gravitational-wave populations: Hierarchical black-hole mergers
• Multi-physics constraints at different densities to probe nuclear symmetry energy in hyperonic neutron stars
• Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910
• Teamwork Makes the Dream Work: Optimizing Multi-Telescope Observations of Gravitational-Wave Counterparts
• Bayesian model-selection of neutron star equation of state using multi-messenger observations
• Eccentric binary black holes: Comparing numerical relativity and small mass-ratio perturbation theory
• Ready-to-use Fourier domain templates for compact binaries inspiraling along moderately eccentric orbits
• Generalized quasi-Keplerian solution for eccentric, non-spinning compact binaries at 4PN order and the associated IMR waveform
• Neutrino emission from binary neutron star mergers: characterizing light curves and mean energies
• Deep-Learning Continuous Gravitational Waves: Multiple detectors and realistic noise
• Generation of squeezed vacuum state in the millihertz frequency band
• Impact of infrasound atmospheric noise on gravity detectors used for astrophysical and geophysical applications
• Impact of eccentricity on the gravitational wave searches for binary black holes: High mass case
• Cosmological Collider Signatures of Massive Vectors from Non-Gaussian Gravitational Waves
• What can we learn from the stochastic gravitational wave background produced by oscillons?
• A new data analysis framework for the search of continuous gravitational wave signals
• A Machine Learning Based Source Property Inference for Compact Binary Mergers
• Current and future constraints on cosmology and modified gravitational wave friction from binary black holes
• Numerical-relativity simulations of long-lived remnants of binary neutron star mergers
• On the identification of individual gravitational wave image types of a lensed system using higher-order modes
• Do unequal-mass binary black hole systems have larger ${\chi }_{\text{eff}}$? Probing correlations with copulas in gravitational-wave astronomy
• The population properties of spinning black holes using Gravitational-wave Transient Catalog 3
• LIGO--Virgo correlations between mass ratio and effective inspiral spin: testing the active galactic nuclei channel
• Testing General Relativity with Gravitational Waves: An Overview
• Black hole induced spins from hyperbolic encounters in dense clusters
• Leveraging waveform complexity for confident detection of gravitational waves
• Impact of astrophysical binary coalescence timescales on the rate of lensed gravitational wave events
• The host galaxies of double compact objects merging in the local Universe
• Constraining the p-mode--g-mode tidal instability with GW170817
• Numerical relativity surrogate model with memory effects and post-Newtonian hybridization
• Real-time gravitational-wave inference for binary neutron stars using machine learning
• Probing the equation of state of neutron star matter with gravitational waves from binary inspirals in light of GW170817: a brief review
• Classifying the unknown: discovering novel gravitational-wave detector glitches using similarity learning
• Detecting a stochastic gravitational-wave background in the presence of correlated magnetic noise
• A scalable random forest regressor for combining neutron-star equation of state measurements: A case study with GW170817 and GW190425
• Spontaneous scalarization: asymmetron as dark matter
• Inferring eccentricity evolution from observations of coalescing binary black holes
• Quiescent and active galactic nuclei as factories of merging compact objects in the era of gravitational-wave astronomy
• Quantifying the Effect of Power Spectral Density Uncertainty on Gravitational-Wave Parameter Estimation for Compact Binary Sources
• The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?
• Ultralight vector dark matter search with auxiliary length channels of gravitational wave detectors
• Three dimensional magnetorotational core-collapse supernova explosions of a 39 solar mass progenitor star
• Stochastic gravitational wave background anisotropies in the mHz band: astrophysical dependencies
• Swift follow-up of gravitational wave triggers: results from the first aLIGO run and optimisation for the future
• Limits of Astrophysics with Gravitational-Wave Backgrounds
• Importance nested sampling with normalising flows
• Standard-siren cosmology using gravitational waves from binary black holes
• Hierarchical Inference of Binary Neutron Star Mass Distribution and Equation of State with Gravitational Waves
• Common-spectrum process versus cross-correlation for gravitational-wave searches using pulsar timing arrays
• Accretion-Induced Collapse of Neutron Stars in the Disks of Active Galactic Nuclei
• Search for a scalar induced stochastic gravitational wave background in the third LIGO-Virgo observing run
• Accuracy of binary black hole waveform models for aligned-spin binaries
• Signatures of mass ratio reversal in gravitational waves from merging binary black holes
• Adding eccentricity to quasicircular binary-black-hole waveform models
• Cosmology with Standard Sirens at Cosmic Noon
• Removing degeneracy and multimodality in gravitational wave source parameters
• Modeling Equal and Unequal Mass Binary Neutron Star Mergers Using Public Codes
• Are Parametrized Tests of General Relativity with Gravitational Waves Robust to Unknown Higher Post-Newtonian Order Effects?
• Pure polarization test of GW170814 and GW170817 using waveforms consistent with modified theories of gravity
• IceCube Search for Neutrinos Coincident with Compact Binary Mergers from LIGO-Virgo's First Gravitational-Wave Transient Catalog
• Search for gravitational waves from the coalescence of sub-solar mass and eccentric compact binaries
• Rapid Identification of Strongly Lensed Gravitational-Wave Events with Machine Learning
• Gravitational waves from first-order phase transitions: Towards model separation by bubble nucleation rate
• Observation of a Correlation Between Internal friction and Urbach Energy in Amorphous Oxides Thin Films
• Astrophysical implications of GW190412 as a remnant of a previous black-hole merger
• Detection and localization of continuous gravitational waves with pulsar timing arrays: the role of pulsar terms
• Detecting stochastic gravitational waves with binary resonance
• Deep Einstein@Home all-sky search for continuous gravitational waves in LIGO O3 public data
• Constraining the neutron-matter equation of state with gravitational waves
• Single field inflation in the light of Pulsar Timing Array Data: Quintessential interpretation of blue tilted tensor spectrum through Non-Bunch Davies initial condition
• Gravitational waves and the polarizations in Hořava gravity after GW170817
• Optimization of seismometer arrays for the cancellation of Newtonian noise from seismic body waves
• Searching for mass-spin correlations in the population of gravitational-wave events: the GWTC-3 case study
• Scalar induced gravity waves from ultra slow-roll Galileon inflation
• Lensing or luck? False alarm probabilities for gravitational lensing of gravitational waves
• Systematic bias on the inspiral-merger-ringdown consistency test due to neglect of orbital eccentricity
• Precision cosmology and the stiff-amplified gravitational-wave background from inflation: NANOGrav, Advanced LIGO-Virgo and the Hubble tension
• Hearing gravity from the cosmos: GWTC-2 probes general relativity at cosmological scales
• Lensed or not lensed: Determining lensing magnifications for binary neutron star mergers from a single detection
• Accurate modeling and mitigation of overlapping signals and glitches in gravitational-wave data
• Constraining extra dimensions using observations of black hole quasi-normal modes
• A search for optical and near-infrared counterparts of the compact binary merger GW190814
• A Rosetta Stone for eccentric gravitational waveform models
• (H)DPGMM: A Hierarchy of Dirichlet Process Gaussian Mixture Models for the inference of the black hole mass function
• X-ray-powered macronovae
• PhaseTracer: tracing cosmological phases and calculating transition properties
• physiCal: A physical approach to the marginalization of LIGO calibration uncertainties
• Detection Prospects of Core-Collapse Supernovae with Supernova-Optimized Third-Generation Gravitational-wave Detectors
• Constraints on planetary and asteroid-mass primordial black holes from continuous gravitational-wave searches
• Tachyonic Preheating in Palatini $R^2$ Inflation
• $\mathtt{bajes}$: Bayesian inference of multimessenger astrophysical data, methods and application to gravitational-waves
• Gravitational Wave observatories may be able to detect hyperbolic encounters of Black Holes
• Low-mass neutron stars: universal relations, the nuclear symmetry energy and gravitational radiation
• Search for gravitational waves from high-mass-ratio compact-binary mergers of stellar mass and sub-solar mass black holes
• Constraints On Scalar-Induced Gravitational Waves Up To Third Order From Joint Analysis of BBN, CMB, And PTA Data
• Validity of common modelling approximations for precessing binary black holes with higher-order modes
• Bayesian Implications for the Primordial Black Holes from NANOGrav's Pulsar-Timing Data Using the Scalar-Induced Gravitational Waves
• Measuring the Hubble constant with black sirens
• A surrogate model for gravitational waveforms of spin-aligned binary black holes with eccentricities
• Convolutional neural networks for the detection of the early inspiral of a gravitational-wave signal
• Parameter-space metric for all-sky semicoherent searches for gravitational-wave pulsars
• Hierarchical multi-stage MCMC follow-up of continuous gravitational wave candidates
• Nucleonic metamodelling in light of multimessenger, PREX-II and CREX data
• Detection of Gravitational Waves Using Bayesian Neural Networks
• Constraints on the binary black hole nature of GW151226 and GW170608 from the measurement of spin-induced quadrupole moments
• Common Envelope Wind Tunnel: The Effects of Binary Mass Ratio and Implications for the Accretion-Driven Growth of LIGO Binary Black Holes
• Directed search for continuous gravitational-wave signals from the Galactic Center in the Advanced LIGO second observing run
• Constraints on the Physical Properties of GW190814 through Simulations based on DECam Follow-up Observations by the Dark Energy Survey
• Towards the routine use of subdominant harmonics in gravitational-wave inference: re-analysis of GW190412 with generation X waveform models
• Binary black hole spectroscopy: a no-hair test of GW190814 and GW190412
• Application of dictionary learning to denoise LIGO's blip noise transients
• Forecasting F(Q) cosmology with $\Lambda$CDM background using standard sirens
• Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars
• Dynamics of binary black holes in low-mass young star clusters
• Robust semicoherent searches for continuous gravitational waves with noise and signal models including hours to days long transients
• Frequency response of space-based interferometric gravitational-wave detectors
• Towards a first design of a Newtonian-noise cancellation system for Advanced LIGO
• Identifying when Precession can be Measured in Gravitational Waveforms
• Resolving Galactic binaries in LISA data using particle swarm optimization and cross-validation
• Template Bank for Compact Binary Coalescence Searches in Gravitational Wave Data: A General Geometric Placement Algorithm
• Gravitational wave population inference with deep flow-based generative network
• Implications of dedicated seismometer measurements on Newtonian-noise cancellation for Advanced LIGO
• Eccentric Gravitational Wave Bursts in the Post-Newtonian Formalism
• On the single-event-based identification of primordial black hole mergers at cosmological distances
• Convective Excitation of Inertial Modes in Binary Neutron Star Mergers
• Gravitational-wave inference in the catalog era: evolving priors and marginal events
• Deep Residual Networks for Gravitational Wave Detection
• $N-$body dynamics of Intermediate mass-ratio inspirals in globular clusters
• Possible golden events for ringdown gravitational waves
• Population properties and multimessenger prospects of neutron star-black hole mergers following GWTC-3
• Flexible and Fast Estimation of Binary Merger Population Distributions with Adaptive KDE
• The Spectroscopic Classification of Astronomical Transients (SCAT) Survey: Overview, Pipeline Description, Initial Results, and Future Plans
• What You Don't Know Can Hurt You: Use and Abuse of Astrophysical Models in Gravitational-wave Population Analyses
• Pre-merger localization of compact-binary mergers with third generation observatories
• Enhancement of primordial curvature perturbations in $R^3$-corrected Starobinsky-Higgs inflation
• Dirichlet Process Gaussian-mixture model: An application to localizing coalescing binary neutron stars with gravitational-wave observations
• Parametrized tests of post-Newtonian theory using principal component analysis
• Prospects of discovering sub-solar primordial black holes using the stochastic gravitational wave background from third-generation detectors
• Normalizing flows as an avenue to study overlapping gravitational wave signals
• Search for Multi-messenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during its first Observing Run, ANTARES and IceCube
• Energy Sources and Light Curves of Macronovae
• Search for black hole hyperbolic encounters with gravitational wave detectors
• Complete conservative dynamics for inspiralling compact binaries with spins at the fourth post-Newtonian order
• The most powerful astrophysical events: Gravitational-wave peak luminosity of binary black holes as predicted by numerical relativity
• Model-Based Cross-Correlation Search for Gravitational Waves from Scorpius X-1
• Limits on hierarchical black hole mergers from the most negative ${\chi }_{\mathrm{eff}}$ systems
• Dynamic Normalization for Compact Binary Coalescence Searches in Non-Stationary Noise
• Exploring the sky localization and early warning capabilities of third generation gravitational wave detectors in three-detector network configurations
• Assessing the Readiness of Numerical Relativity for LISA and 3G Detectors
• Inferring the lensing rate of LIGO-Virgo sources from the stochastic gravitational wave background
• GW170817A as a Hierarchical Black Hole Merger
• Using Deep Learning to Localize Gravitational Wave Sources
• Swift-XRT follow-up of gravitational wave triggers during the third aLIGO/Virgo observing run
• Single- versus two-parameter Fisher information in quantum interferometry
• Heavy double neutron stars: birth, mid-life and death
• Exploring the hidden Universe: A novel phenomenological approach for recovering arbitrary gravitational-wave millilensing configurations
• Bayesian nonparametric spectral density estimation using B-spline priors
• Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA
• New binary black hole mergers in the LIGO-Virgo O3b data
• Subtracting Compact Binary Foregrounds to Search for Subdominant Gravitational-Wave Backgrounds in Next-Generation Ground-Based Observatories
• Spin it as you like: the (lack of a) measurement of the spin tilt distribution with LIGO-Virgo-KAGRA binary black holes
• Global numerical simulations of the rise of vortex-mediated pulsar glitches in full general relativity
• Probing the progenitors of spinning binary black-hole mergers with long gamma-ray bursts
• Measuring the spins of heavy binary black holes
• Testing general relativity with gravitational-wave catalogs: the insidious nature of waveform systematics
• Structure and morphology of low mechanical loss TiO${}_2$-doped Ta${}_2$O${}_5$
• High-Reflection Coatings for Gravitational-Wave Detectors: State of The Art and Future Developments
• Cross-correlating dark sirens and galaxies: constraints on $H_0$ from GWTC-3 of LIGO-Virgo-KAGRA
• Blind spots and biases: the dangers of ignoring eccentricity in gravitational-wave signals from binary black holes
• Tail contributions to gravitational conservative dynamics
• Growth of accretion driven scalar hair around Kerr black holes
• Astronomical Distance Determination in the Space Age. Secondary distance indicators
• Measuring neutron star tidal deformability with Advanced LIGO: a Bayesian analysis of neutron star - black hole binary observations
• Distinguishing black-hole spin-orbit resonances by their gravitational wave signatures. II: Full parameter estimation
• Quantum-enhanced interferometry for axion searches
• Newtonian-noise cancellation in full-tensor gravitational-wave detectors
• Parameter Estimation Bias From Overlapping Binary Black Hole Events In Second Generation Interferometers
• Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
• Impacts of overlapping gravitational-wave signals on the parameter estimation: Toward the search for cosmological backgrounds
• Third post-Newtonian effective-one-body Hamiltonian in scalar-tensor and Einstein-scalar-Gauss-Bonnet gravity
• Fast, faithful, frequency-domain effective-one-body waveforms for compact binary coalescences
• First search for long-duration transient gravitational waves after glitches in the Vela and Crab pulsars
• Unveiling the merger structure of black hole binaries in generic planar orbits
• Baryon and Lepton Number Violation from Gravitational Waves
• Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries
• Generation of very high-order high purity Gaussian modes via spatial light modulation
• Assessing the model waveform accuracy of gravitational waves
• Resonant Excitation of Quasinormal Modes of Black Holes
• Probing Quarkyonic Matter in Neutron Stars with the Bayesian Nuclear-Physics Multi-Messenger Astrophysics Framework
• Gravitational waves from the first order phase transition of the Higgs field at high energy scales
• Inferring Astrophysical Parameters of Core-Collapse Supernovae from their Gravitational-Wave Emission
• Compact Michelson interferometers with subpicometer sensitivity
• Primordial non-Gaussianity as a saviour for PBH overproduction in SIGWs generated by Pulsar Timing Arrays for Galileon inflation
• Measuring binary black hole orbital-plane spin orientations
• Viewing angle of binary neutron star mergers
• The orbit of GW170817 was inclined by less than 28 degrees to the line of sight
• Optimal Mach-Zehnder phase sensitivity with Gaussian states
• Searching for ringdown higher modes with a numerical relativity-informed post-merger model
• Gravitational-wave Merger Forecasting: Scenarios for the early detection and localization of compact-binary mergers with ground based observatories
• Search for Kilogram-scale Dark Matter with Precision Displacement Sensors
• Machine learning for gravitational-wave detection: surrogate Wiener filtering for the prediction and optimized cancellation of Newtonian noise at Virgo
• Evidence for the evolution of black hole mass function with redshift
• GRB/GW association: Long-short GRB candidates, time-lag, measuring gravitational wave velocity and testing Einstein's equivalence principle
• Poking Holes: Looking for Gaps in LIGO/Virgo's Black Hole Population
• Measuring the properties of active galactic nuclei disks with gravitational waves
• Tiling strategies for optical follow-up of gravitational wave triggers by wide field of view telescopes
• Spin and Eccentricity Evolution in Triple Systems: from the Lidov-Kozai Interaction to the Final Merger of the Inner Binary
• The Eccentric Behavior of Inspiraling Compact Binaries
• Second Einstein Telescope Mock Data and Science Challenge: Low Frequency Binary Neutron Star Data Analysis
• Localization of binary mergers with gravitational-wave detectors of second and third generation
• Fusing numerical relativity and deep learning to detect higher-order multipole waveforms from eccentric binary black hole mergers
• Fermi GBM Observations of GRB 150101B: A Second Nearby Event with a Short Hard Spike and a Soft Tail
• Evolution of Retrograde Orbiters in an AGN Disk
• Effective-One-Body Numerical-Relativity waveform model for Eccentric spin-precessing binary black hole coalescence
• Gravitational wave propagation beyond geometric optics
• Improving the background of gravitational-wave searches for core collapse supernovae: A machine learning approach
• Inferring fundamental spacetime symmetries with gravitational-wave memory: from LISA to the Einstein Telescope
• Label Switching Problem in Bayesian Analysis for Gravitational Wave Astronomy
• Inspiral-merger-ringdown waveforms in Einstein-scalar-Gauss-Bonnet gravity within the effective-one-body formalism
• New effective precession spin for modeling multimodal gravitational waveforms in the strong-field regime
• High-power all-fiber ultra-low noise laser
• Early warning of coalescing neutron-star and neutron-star-black-hole binaries from nonstationary noise background using neural networks
• Implementing a semicoherent search for continuous gravitational waves using optimally-constructed template banks
• The observed mass distribution of Galactic black hole LMXBs is biased against massive black holes
• Improved statistic to identify strongly lensed gravitational wave events
• A wider look at the gravitational-wave transients from GWTC-1 using an unmodeled reconstruction method
• Search for gravitational waves from Scorpius X-1 with a hidden Markov model in O3 LIGO data
• Friction on ALP domain walls and gravitational waves
• Distinguishing high-mass binary neutron stars from binary black holes with second- and third-generation gravitational wave observatories
• Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): Observations and Analysis from Advanced LIGO/Virgo's Third Observing Run
• Searching for anisotropy in the distribution of binary black hole mergers
• A Search for Gravitational Waves from Binary Mergers with a Single Observatory
• Translating neutron star observations to nuclear symmetry energy via artificial neural networks
• Mapping the Gravitational-wave Sky with LISA: A Bayesian Spherical Harmonic Approach
• Stochastic gravitational wave background: methods and Implications
• Merger rate of stellar black hole binaries above the pair instability mass gap
• R-mode astronomy
• Passive, free-space laser gyroscope
• The initial value problem as it relates to numerical relativity
• NuRIA: Numerical Relativity Injection Analysis of spinning binary black hole signals in Advanced LIGO data
• Evidence for a correlation between binary black hole mass ratio and black-hole spins
• Quantum expander for gravitational-wave observatories
• Finite tidal effects in GW170817: Observational evidence or model assumptions?
• X-ray guided gravitational-wave search for binary neutron star merger remnants
• IceCube search for neutrinos coincident with gravitational wave events from LIGO/Virgo run O3
• Angular emission patterns of remnant black holes
• Archival searches for stellar-mass binary black holes in LISA
• Pulsars probe the low-frequency gravitational sky: Pulsar Timing Arrays basics and recent results
• Prospects for multi-messenger detection of binary neutron star mergers in the fourth LIGO-Virgo-KAGRA observing run
• The ${\chi }_{\mathrm{eff}}-z$ correlation of field binary black hole mergers and how 3G gravitational-wave detectors can constrain it
• Excitation of f-modes during mergers of spinning binary neutron star
• Impact of the tidal p-g instability on the gravitational wave signal from coalescing binary neutron stars
• Intensity and anisotropies of the stochastic Gravitational Wave background from merging compact binaries in galaxies
• Systematic errors in estimation of gravitational-wave candidate significance
• Astrophysics with core-collapse supernova gravitational wave signals in the next generation of gravitational wave detectors
• Model-independent test of the parity symmetry of gravity with gravitational waves
• Estimation of losses in a 300 m filter cavity and quantum noise reduction in the KAGRA gravitational-wave detector
• Sensitivity functions for space-borne gravitational wave detectors
• Neutron star binary orbits in their host potential: effect on early r-process enrichment
• Multiband Gravitational Wave Parameter Estimation: A Study of Future Detectors
• Cosmic Evolution of Stellar-mass Black Hole Merger Rate in Active Galactic Nuclei
• The Unprecedented Properties of the First Electromagnetic Counterpart to a Gravitational Wave Source
• Cosmography using strongly lensed gravitational waves from binary black holes
• From One to Many: A Deep Learning Coincident Gravitational-Wave Search
• Deep Learning Detection and Classification of Gravitational Waves from Neutron Star-Black Hole Mergers
• Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations
• Relativistic effective action of dynamical gravitomagnetic tides for slowly rotating neutron stars
• All-sky, all-frequency directional search for persistent gravitational-waves from Advanced LIGO's and Advanced Virgo's first three observing runs
• Methods for the detection of gravitational waves from sub-solar mass ultracompact binaries
• Hereditary Effects in Eccentric Compact Binary Inspirals to Third Post-Newtonian Order
• Gravitational wave forms, polarizations, response functions and energy losses of triple systems in Einstein-Aether theory
• Constraining early dark energy with gravitational waves before recombination
• Numerical investigation of plasma-driven superradiant instabilities
• Detection and parameter estimation challenges of Type-II lensed binary black hole signals
• GW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-Spin Black Hole Coalescence
• Probing the Black Hole Metric. I. Black Hole Shadows and Binary Black-Hole Inspirals
• Hierarchical binary black hole mergers in globular clusters: mass function and evolution with redshift
• Can the gravitational wave background feel wiggles in spacetime?
• SOAP: A generalised application of the Viterbi algorithm to searches for continuous gravitational-wave signals
• Challenges and Opportunities of Gravitational Wave Searches above 10 kHz
• Quadratic-in-spin interactions at fifth post-Newtonian order probe new physics
• The Quadrupole Moment of Compact Binaries to the Fourth post-Newtonian Order: From Source to Canonical Moment
• New equation of states for postmerger supramassive quark stars
• Detectability of kilonovae in optical surveys: $post$-$mortem$ examination of the LVC O3 run follow-up
• Faint objects in motion: the new frontier of high precision astrometry
• Comprehensive analysis of the tidal effect in gravitational waves and implication for cosmology
• Probing Extremal Gravitational-Wave Events with Coarse-Grained Likelihoods
• lensingGW: a Python package for lensing of gravitational waves
• The host galaxies of double compact objects across cosmic time
• Ringdown frequencies in black holes formed from precessing black-hole binaries
• Inferring the core-collapse supernova explosion mechanism with three-dimensional gravitational-wave simulations
• All-sky search for long-duration gravitational wave transients with LIGO
• On the Potential Observation of False Deviations from General Relativity in Gravitational Wave Observations from Binary Black Holes
• Reconstructing gravitational wave signals from binary black hole mergers with minimal assumptions
• First search for ultralight dark matter with a space-based gravitational-wave antenna: LISA Pathfinder
• Impact of Schumann resonances on the Einstein Telescope and projections for the magnetic coupling function
• Optical follow-up of gravitational wave events during the second advanced LIGO/VIRGO observing run with the DLT40 Survey
• Inferring the neutron star maximum mass and lower mass gap in neutron star-black hole systems with spin
• Spin-Precessing Black Hole Binaries in Dynamical Chern-Simons Gravity
• A brief history of gravitational wave research
• Exploring the Impact of Microlensing on Gravitational Wave Signals: Biases, Population Characteristics, and Prospects for Detection
• Cosmography with next-generation gravitational wave detectors
• Probing new light gauge bosons with gravitational-wave interferometers using an adapted semi-coherent method
• Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution
• VARAHA: A Fast Non-Markovian sampler for estimating Gravitational-Wave posteriors
• Testing the multipole structure and conservative dynamics of compact binaries using gravitational wave observations: The spinning case
• Systematic errors in estimation of gravitational-wave candidate significance
• Axion dark matter search using arm cavity transmitted beams of gravitational wave detectors
• Refined clock-jitter reduction in the Sagnac-type time-delay interferometry combinations
• Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models
• Probing cosmological fields with gravitational wave oscillations
• Fourth post-Newtonian effective-one-body Hamiltonians with generic spins
• A gravitational-wave limit on the Chandrasekhar mass of dark matter
• Testing Gravity with Gravitational Wave Source Counts
• Gravitational waves from extreme mass ratio inspirals around bumpy black holes
• Compact binary coalescences: Constraints on waveforms
• Stellar-mass black holes in young massive and open stellar clusters V: comparisons with LIGO-Virgo merger rate densities
• High Quality QCD Axion at Gravitational Wave Observatories
• Estimating parameters of binary black holes from gravitational-wave observations of their inspiral, merger and ringdown
• Bayesian Multi-Messenger Search Method for Common Sources of Gravitational Waves and High-Energy Neutrinos
• Measuring stochastic gravitational-wave energy beyond general relativity
• Globally coherent short duration magnetic field transients and their effect on ground based gravitational-wave detectors
• Probing lens-induced gravitational-wave birefringence as a test of general relativity
• Regression methods in waveform modeling: a comparative study
• Black Hole Leftovers: The Remnant Population from Binary Black Hole Mergers
• Accelerating multimodal gravitational waveforms from precessing compact binaries with artificial neural networks
• Effect of spin on the inspiral of binary neutron stars
• Inferring the maximum and minimum mass of merging neutron stars with gravitational waves
• Evading no-go for PBH formation and production of SIGWs using Multiple Sharp Transitions in EFT of single field inflation
• ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes
• Cosmology with the Einstein Telescope: No Slip Gravity Model and Redshift Specifications
• Systematic analysis of the impacts of symmetry energy parameters on neutron star properties
• Detectability of Gravitational Waves from the Coalescence of Massive Primordial Black Holes with Initial Clustering
• Observing an intermediate mass black hole GW190521 with minimal assumptions
• Assessing the compact-binary merger candidates reported by the MBTA pipeline in the LIGO-Virgo O3 run: probability of astrophysical origin, classification, and associated uncertainties
• Gravitational wave signature of proto-neutron star convection: I. MHD numerical simulations
• Prospects for gravitational-wave polarization test from compact binary mergers with future ground-based detectors
• Comprehensive study of amorphous metal oxide and Ta${}_2$O${}_5$-based mixed oxide coatings for gravitational-wave detectors
• Stars stripped in binaries -- the living gravitational wave sources
• Core collapse in massive scalar-tensor gravity
• Gravitational waveforms for neutron star binaries from binary black hole simulations
• Radiation-Pressure-Mediated Control of an Optomechanical Cavity
• Binary Neutron Stars Gravitational Wave Detection Based on Wavelet Packet Analysis And Convolutional Neural Networks
• A paradigm of warm quintessential inflation and production of relic gravity waves
• Population Properties of Gravitational-Wave Neutron Star--Black Hole Mergers
• Optimization of model independent gravitational wave search using machine learning
• Anomaly Detection in Gravitational Waves data using Convolutional AutoEncoders
• Search for gravitational waves from five low mass X-ray binaries in the second Advanced LIGO observing run with an improved hidden Markov model
• Leveraging gravitational-wave memory to distinguish neutron star--black hole binaries from black hole binaries
• Characterizing Earth gravity field fluctuations with the MIGA antenna for future Gravitational Wave detectors
• Ultra-precision quantum sensing and measurement based on nonlinear hybrid optomechanical systems containing ultracold atoms or atomic Bose-Einstein condensate
• Generalized Approach to Matched Filtering using Neural Networks
• Constraining cosmological extra dimensions with gravitational wave standard sirens: from theory to current and future multi-messenger observations
• Optical and mechanical properties of ion-beam-sputtered Nb${}_2$O${}_5$ and TiO${}_2$-Nb${}_2$O${}_5$ thin films for gravitational-wave interferometers
• Resolving Galactic binaries using a network of space-borne gravitational wave detectors
• Numerical-Relativity-Informed Effective-One-Body model for Black-Hole-Neutron-Star Mergers with Higher Modes and Spin Precession
• Quantifying modeling uncertainties when combining multiple gravitational-wave detections from binary neutron star sources
• Impact of correlated magnetic noise on the detection of stochastic gravitational waves: Estimation based on a simple analytical model
• Optimizing spinning time-domain gravitational waveforms for Advanced LIGO data analysis
• Have Pulsar Timing Arrays detected the Hot Big Bang? Gravitational Waves from Strong First Order Phase Transitions in the Early Universe
• Mapping the Universe Expansion: Enabling percent-level measurements of the Hubble Constant with a single binary neutron-star merger detection
• A Channel to Form Fast-spinning Black Hole--Neutron Star Binary Mergers as Multi-messenger Sources
• Source properties of the lowest signal-to-noise-ratio binary black hole detections
• Transient gravitational waves from pulsar post-glitch recoveries
• Inference-optimized AI and high performance computing for gravitational wave detection at scale
• Gravitational Waves from Core-Collapse Supernovae
• Classifying the Equation of State from Rotating Core Collapse Gravitational Waves with Deep Learning
• Direct determination of supermassive black hole properties with gravitational-wave radiation from surrounding stellar-mass black hole binaries
• Light curve classification with recurrent neural networks for GOTO: dealing with imbalanced data
• LSTM and CNN application for core-collapse supernova search in gravitational wave real data
• Search for gravitational-wave bursts in the third Advanced LIGO-Virgo run with coherent WaveBurst enhanced by Machine Learning
• Bayesian semiparametric power spectral density estimation with applications in gravitational wave data analysis
• Constraining modified theories of gravity with gravitational wave stochastic background
• Spectral Cauchy-characteristic extraction of the gravitational wave news function
• Measuring the Speed of Gravitational Waves from the First and Second Observing Run of Advanced LIGO and Advanced Virgo
• The detection of Quasinormal Mode of Pop III Binary Black Hole merger with final $M\sim 60M_{\odot }$ and $a/M\sim 0.7$ would confirm the strong gravity space-time around $\sim 2M$ which is only $\sim 1.17$ times the event horizon radius
• Strange stars in $f(\mathcal{R})$ gravity Palatini formalism and gravitational wave echoes from them
• Investigation of the effects of non-Gaussian noise transients and their mitigation in parameterized gravitational-wave tests of general relativity
• Parameterised population models of transient non-Gaussian noise in the LIGO gravitational-wave detectors
• Binary White Dwarfs as Laboratories for Extreme Gravity with LISA
• Parameter estimation for strong phase transitions in supranuclear matter using gravitational-wave astronomy
• High sensitivity, levitated microsphere apparatus for short-distance force measurements
• Full analytical formulas for frequency response of space-based gravitational wave detectors
• Ringdown amplitudes of nonspinning eccentric binaries
• Combining effective-one-body accuracy and reduced-order-quadrature speed for binary neutron star merger parameter estimation with machine learning
• pygwb: Python-based library for gravitational-wave background searches
• Gravitational wave populations and cosmology with neural posterior estimation
• Waltzing binaries: Probing line-of-sight acceleration of merging compact objects with gravitational waves
• Stochastic Gravitational Wave Background and Eccentric Stellar Compact Binaries
• Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution
• Parametrizing gravitational-wave polarizations
• J-GEM Follow-Up Observations to Search for an Optical Counterpart of The First Gravitational Wave Source GW150914
• Systematic challenges for future gravitational wave measurements of precessing binary black holes
• Recommended high performance telescope system design for the TianQin project
• Large fluctuations and Primordial Black Holes
• Eccentricity-induced systematic error on parametrized tests of general relativity: Hierarchical Bayesian inference applied to a binary black hole population
• Understanding how fast black holes spin by analysing data from the second gravitational-wave catalogue
• Interplay of spin-precession and higher harmonics in the parameter estimation of binary black holes
• GW190521: tracing imprints of spin-precession on the most massive black hole binary
• Improving significance of binary black hole mergers in Advanced LIGO data using deep learning : Confirmation of GW151216
• An Infrared Search for Kilonovae with the WINTER Telescope. I. Binary Neutron Star Mergers
• Resolving the eccentricity of stellar mass binary black holes with next generation ground-based gravitational wave detectors
• Gravity Spy: Lessons Learned and a Path Forward
• Phase-coherent mapping of gravitational-wave backgrounds using ground-based laser interferometers
• J-GEM Follow-Up Observations of The Gravitational Wave Source GW151226
• Constraint on the ejecta mass for a black hole-neutron star merger event candidate S190814bv
• Prospects of gravitational-waves detections from common-envelope evolution with LISA
• Inferring the population properties of binary black holes from unresolved gravitational waves
• The quasi normal modes of growing dirty black holes
• Frequency-domain waveform approximants capturing Doppler shifts
• Petrov Type, Principal Null Directions, and Killing Tensors of Slowly-Rotating Black Holes in Quadratic Gravity
• Fiducial displacements with improved accuracy for the global network of gravitational wave detectors
• Reconstructing the Genealogy of LIGO-Virgo Black Holes
• Searching for parity violation with the LIGO-Virgo-KAGRA network
• Exploration of co-sputtered Ta${}_2$O${}_5$-ZrO${}_2$ thin films for gravitational-wave detectors
• Neutron star-black hole mergers in next generation gravitational-wave observatories
• Probing elastic quark phases in hybrid stars with radius measurements
• Frequency-Domain Analysis of Black-Hole Ringdowns
• Constraints on compact binary merger evolution from spin-orbit misalignment in gravitational-wave observations
• A morphology-independent test of the mixed polarization content of gravitational wave signals from compact binary coalescences
• Gravitational Wave Signals from Two-Dimensional Core-Collapse Supernova Models with Rotation and Magnetic Fields
• Template bank for compact binary mergers in the fourth observing run of Advanced LIGO, Advanced Virgo, and KAGRA
• Quantum Gravitational Sensor for Space Debris
• Enhancing confidence in the detection of gravitational waves from compact binaries using signal coherence
• The minimum and maximum gravitational-wave background from supermassive binary black holes
• An optimized PyCBC search for gravitational waves from intermediate-mass black hole mergers
• Fast post-adiabatic waveforms in the time domain: Applications to compact binary coalescences in LIGO and Virgo
• Model-based cross-correlation search for gravitational waves from the low-mass X-ray binary Scorpius X-1 in LIGO O3 data
• Swift/UVOT follow-up of Gravitational Wave Alerts in the O3 era
• Modified gravitational wave propagation with higher modes and its degeneracies with lensing
• Higher-order Hermite-Gauss modes as a robust flat beam in interferometric gravitational wave detectors
• Analysis of a subsolar-mass compact binary candidate from the second observing run of Advanced LIGO
• Scalable, symmetric atom interferometer for infrasound gravitational wave detection
• The Gravitational Wave Universe Toolbox: A software package to simulate observation of the Gravitational Wave Universe with different detectors
• A robust machine learning algorithm to search for continuous gravitational waves
• The most luminous AGN do not produce the majority of the detected stellar-mass black hole binary mergers in the local Universe
• Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures
• Observable signatures of stellar-mass black holes in active galactic nuclei
• An autoencoder neural network integrated into gravitational-wave burst searches to improve the rejection of noise transients
• Towards establishing the presence or absence of horizons in coalescing binaries of compact objects by using their gravitational wave signals
• Pre-merger alert to detect the very-high-energy prompt emission from binary neutron-star mergers: Einstein Telescope and Cherenkov Telescope Array synergy
• Characterization of binary black holes by heterogeneous gravitational-wave networks
• A study of the Inspiral-Merger-Ringdown Consistency Test with gravitational-wave signals from compact binaries in eccentric orbits
• Spin effects in Spherical Harmonic Modes of Gravitational Waves from Eccentric Compact Binary Inspirals
• Characterizing the observation bias in gravitational-wave detections and finding structured population properties
• Sublunar-Mass Primordial Black Holes from Closed Axion Domain Walls
• Searching for Cross-Correlation Between Stochastic Gravitational Wave Background and Galaxy Number Counts
• Scalar-tensor mixed polarization search of gravitational waves
• The binary-host connection: astrophysics of gravitational wave binaries from their host galaxy properties
• Engineering the Optical Spring via Intra-Cavity Optical-Parametric Amplification
• Accelerating Multi-Model Bayesian Inference, Model Selection and Systematic Studies for Gravitational Wave Astronomy
• Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
• Can we decipher the composition of the core of a neutron star?
• Is there an excess of black holes around $20M_{\odot }$? Optimising the complexity of population models with the use of reversible jump MCMC
• Universal features of gravitational waves emitted by superkick binary black hole systems
• Observation of eccentric binary black hole mergers with second and third generation gravitational wave detector networks
• Model exploration in gravitational-wave astronomy with the maximum population likelihood
• Dropping Anchor: Understanding the Populations of Binary Black Holes with Random and Aligned Spin Orientations
• Observing Gravitational Waves with a Single Detector
• Triaxially-deformed Freely-precessing Neutron Stars: Continuous electromagnetic and gravitational radiation
• Accurate and Efficient Waveform Model for Precessing Binary Black Holes
• Binary black hole mergers from young massive clusters in the pair-instability supernova mass gap
• Application of a hierarchical MCMC follow-up to Advanced LIGO continuous gravitational-wave candidates
• Observation of the Three-Mode Parametric Instability
• Combining Post-Circular and Padé approximations to compute Fourier domain templates for eccentric inspirals
• Mitigating mode-matching loss in nonclassical laser interferometry
• ETpathfinder: a cryogenic testbed for interferometric gravitational-wave detectors
• Gravitational Waves as a Probe of Globular Cluster Formation and Evolution
• Mechanical Ringdown Studies of Large-Area Substrate-Transferred GaAs/AlGaAs Crystalline Coatings
• Astrophysical Gravitational-Wave Echoes from Galactic Nuclei
• Charged Black Hole Mergers: Orbit Circularisation and Chirp Mass Bias
• Limiting the effects of earthquakes on gravitational-wave interferometers
• Statistical and systematic uncertainties in extracting the source properties of neutron star - black hole binaries with gravitational waves
• Analyzing black-hole ringdowns
• The population of merging compact binaries inferred using gravitational waves through GWTC-3
• The Redshift Evolution of the Binary Black Hole Mass Distribution from Dense Star Clusters
• Frequency response of time-delay interferometry for space-based gravitational wave antennas
• Simulating Transient Noise Bursts in LIGO with Generative Adversarial Networks
• Gravitational wave inference on a numerical-relativity simulation of a black hole merger beyond general relativity
• Measurability of precession and eccentricity for heavy binary-black-hole mergers
• Mergers of black hole-neutron star binaries and rates of associated electromagnetic counterparts
• Searching for scalar field dark matter with LIGO
• Distinguishing double neutron star from neutron star-black hole binary populations with gravitational wave observations
• Bayesian inference of multimessenger astrophysical data: Joint and coherent inference of gravitational waves and kilonovae
• Constraining Unmodeled Physics with Compact Binary Mergers from GWTC-1
• Eccentricity distributions of eccentric binary black holes in galactic nuclei
• First Tests of a Newtonian Calibrator on an Interferometric Gravitational Wave Detector
• Methods and prospects for gravitational wave searches targeting ultralight vector boson clouds around known black holes
• Optimizing Serendipitous Detections of Kilonovae: Cadence and Filter Selection
• Sensitivity of Space-based Gravitational-Wave Interferometers to Ultralight Bosonic Fields and Dark Matter
• Gravitational wave emission under general parametrized metric from extreme mass ratio inspirals
• Modeling gravitational waves from exotic compact objects
• Black hole science with the Laser Interferometer Space Antenna
• Near and far zone in two-body dynamics: an effective field theory perspective
• Reduction of Classical Measurement Noise via Quantum-Dense Metrology
• Bekenstein-Hod Universal Bound on Information Emission Rate Is Obeyed by LIGO-Virgo Binary Black Hole Remnants
• Measuring tidal effects with the Einstein Telescope: A design study
• Early Warnings of Binary Neutron Star Coalescence using the SPIIR Search
• On the detection and precise localisation of merging black holes events through strong gravitational lensing
• The Missing Link Between Black Holes in High-Mass X-ray Binaries and Gravitational-Wave Sources: Observational Selection Effects
• Eccentric Binary Black Holes with Spin via the Direct Integration of the Post-Newtonian Equations of Motion
• Model-Independent Radiative Symmetry Breaking and Gravitational Waves
• Gravitational Lensing of Gravitational Waves: Probability of Microlensing in Galaxy-Scale Lens Population
• Gravitational wave echoes from compact stars in $f(\mathcal{R},T)$ gravity
• Correlated magnetic noise from anisotropic lightning sources and the detection of stochastic gravitational waves
• Observing binary black hole ringdowns by advanced gravitational wave detectors
• Identification of Binary Neutron Star Mergers in Gravitational-Wave Data Using YOLO One-Shot Object Detection
• Primordial black holes from cusp collapse on cosmic strings
• PyFstat: a Python package for continuous gravitational-wave data analysis
• Prospects for detecting gravitational waves from eccentric subsolar mass compact binaries
• Evidence for subdominant multipole moments and precession in merging black-hole-binaries from GWTC-2.1
• Addressing the challenges of detecting time-overlapping compact binary coalescences
• Binary vision: The merging black hole binary mass distribution via iterative density estimation
• The first five years of gravitational-wave astrophysics
• Induced Gravitational Waves probing Primordial Black Hole Dark Matter with Memory Burden
• Including mode mixing in a higher-multipole model for gravitational waveforms from nonspinning black-hole binaries
• Fortifying gravitational-wave tests of general relativity against astrophysical assumptions
• Measuring the ringdown scalar polarization of gravitational waves in Einstein scalar Gauss-Bonnet gravity
• Identification of Lensed Gravitational Waves with Deep Learning
• Improved analysis of GW190412 with a precessing numerical relativity surrogate waveform model
• Detecting resonant tidal excitations of Rossby modes in coalescing neutron-star binaries with third-generation gravitational-wave detectors
• Which black hole is spinning? Probing the origin of black-hole spin with gravitational waves
• Measuring the properties of nearly extremal black holes with gravitational waves
• Polarized kilonovae from black hole-neutron star mergers
• Improving the absolute accuracy of the gravitational wave detectors by combining the photon pressure and gravity field calibrators
• Implications of comprehensive nuclear and astrophysics data on the equations of state of neutron star matter
• PixelPop: High Resolution Nonparameteric Inference of Gravitational-Wave Populations in Multiple Dimensions
• New Gravitational Wave Discoveries Enabled by Machine Learning
• Unraveling information about supranuclear-dense matter from the complete binary neutron star coalescence process using future gravitational-wave detector networks
• AGILE Observations of the Gravitational-wave Source GW170817: Constraining Gamma-Ray Emission from a NS-NS Coalescence
• Impact of precession on aligned-spin searches for neutron-star--black-hole binaries
• Empirically estimating the distribution of the loudest candidate from a gravitational-wave search
• Baryogenesis in the paradigm of quintessential inflation
• Empirically extending the range of validity of parameter-space metrics for all-sky searches for gravitational-wave pulsars
• Are stellar--mass binary black hole mergers isotropically distributed?
• Searching for New Physics in Ultradense Environment: a Review on Dark Matter Admixed Neutron Stars
• Population inference of spin-induced quadrupole moments as a probe for non-black hole compact binaries
• Prospects for improving the sensitivity of the cryogenic gravitational wave detector KAGRA
• Characterization of numerical relativity waveforms of eccentric binary black hole mergers
• A Direct Approach for the Fluctuation-Dissipation Theorem under Non-Equilibrium Steady-State Conditions
• Progenitors of low-mass binary black-hole mergers in the isolated binary evolution scenario
• Detectability of Gravitational Waves from High-Redshift Binaries
• Maximizing the Probability of Detecting an Electromagnetic Counterpart of Gravitational-wave Events
• Quantum black hole spectroscopy: probing the quantum nature of the black hole area using LIGO-Virgo ringdown detections
• The Return of GOLUM: Improving Distributed Joint Parameter Estimation for Strongly-Lensed Gravitational Waves
• A Gravitational Wave Detector for Post Merger Neutron Stars: Beyond the Quantum Loss Limit of Michelson Fabry Perot Interferometer
• Detection of scalar fields by Extreme Mass Ratio Inspirals with a Kerr black hole
• Cosmography with Standard Sirens from the Einstein Telescope
• Theory-agnostic framework for inspiral tests of general relativity with higher-harmonic gravitational waves
• Presto-Color: A Photometric Survey Cadence for Explosive Physics & Fast Transients
• Detecting the stochastic gravitational wave background with the TianQin detector
• Nonparametric analysis of correlations in the binary black hole population with LIGO-Virgo-KAGRA data
• Bayesian parameter-estimation of Galactic binaries in LISA data with Gaussian Process Regression
• The short gamma-ray burst population in a quasi-universal jet scenario
• Gravitational wave detection without boot straps: a Bayesian approach
• Gravitational-wave inference for eccentric binaries: the argument of periapsis
• Utilizing Gaussian mixture models in all-sky searches for short-duration gravitational wave bursts
• Correlated 1-1000 Hz magnetic field fluctuations from lightning over earth-scale distances and their impact on gravitational wave searches
• Tachyonic Preheating in Plateau Inflation
• Gravitational-Wave Background from Binary Mergers and Metallicity Evolution of Galaxies
• A search for the afterglows, kilonovae, and host galaxies of two short GRBs: GRB 211106A and GRB 211227A
• Sharpening the dark matter signature in gravitational waveforms I: Accretion and eccentricity evolution
• Searching for High Frequency Gravitational Waves with Phonons
• Fast Parameter Estimation of Binary Mergers for Multimessenger Followup
• Lightning-Fast Gravitational Wave Parameter Inference through Neural Amortization
• Search strategies for long gravitational-wave transients: hidden Markov model tracking and seedless clustering
• The permanent ellipticity of the neutron star in PSR J1023+0038
• LISA stellar-mass black hole searches with semicoherent and particle-swarm methods
• Detectability of lensed gravitational waves in matched-filtering searches
• The payload of the Lunar Gravitational-wave Antenna
• Assessing and marginalizing over compact binary coalescence waveform systematics with RIFT
• Applications of machine learning in gravitational wave research with current interferometric detectors
• The MBTA Pipeline for Detecting Compact Binary Coalescences in the Fourth LIGO-Virgo-KAGRA Observing Run
• Adapting to noise distribution shifts in flow-based gravitational-wave inference
• Observational Selection Effects with Ground-based Gravitational Wave Detectors
• Gravitational wave probes of particle dark matter: a review
• Orbital eccentricity in a neutron star - black hole merger
• Gaussian Processes for Glitch-robust Gravitational-wave Astronomy
• Gravitational waves from dark matter collapse in a star
• Search for binary black hole mergers in the third observing run of Advanced LIGO-Virgo using coherent WaveBurst enhanced with machine learning
• Detecting gravitational lensing in hierarchical triples in galactic nuclei with space-borne gravitational-wave observatories
• On the Angular Momentum Transport Efficiency within the Star Constrained from Gravitational-wave Observations
• On Trapped Modes In Variable White Dwarfs As Probes Of The ${}^{12}$C($\alpha ,\gamma$)${}^{16}$O Reaction Rate
• Utilizing the null stream of the Einstein Telescope
• Time-dependent stellar-mass binary black hole mergers in AGN disks: Mass distribution of hierarchical mergers
• The Virgo O3 run and the impact of the environment
• A frequency resolved atlas of the sky in continuous gravitational waves
• Generating transient noise artifacts in gravitational-wave detector data with generative adversarial networks
• Technology for the next gravitational wave detectors
• Efficient parameter inference for gravitational wave signals in the presence of transient noises using temporal and time-spectral fusion normalizing flow
• Constraining gravitational wave amplitude birefringence with GWTC-3
• Parameter estimation methods for analyzing overlapping gravitational wave signals in the third-generation detector era
• A compact instrument for gamma-ray burst detection on a CubeSat platform I: Design drivers and expected performance
• Parameter estimation of a two-component neutron star model with spin wandering
• Gravitational Wave Signatures of Lepton Universality Violation
• Convolutional Neural Networks for the classification of glitches in gravitational-wave data streams
• Identifying correlations between LIGO's astronomical range and auxiliary sensors using lasso regression
• Updated detection prospects for relic neutrinos using coherent scattering
• Daily monitoring of scattered light noise due to microseismic variability at the Virgo interferometer
• Unmodelled Clustering Methods for Gravitational Wave Populations of Compact Binary Mergers
• Unsupervised Learning Architecture for Classifying the Transient Noise of Interferometric Gravitational-wave Detectors
• Distinguishing binary neutron star from neutron star-black hole mergers with gravitational waves
• Cryogenic suspension design for a kilometer-scale gravitational-wave detector
• A Joint Fermi-GBM and LIGO/Virgo Analysis of Compact Binary Mergers From the First and Second Gravitational-wave Observing Runs
• Gravitational wave source populations: Disentangling an AGN component
• Quantum-enhanced super-sensitivity of Mach-Zehnder interferometer using squeezed Kerr state
• The Kitt Peak Electron Multiplying CCD demonstrator
• Estimation of starting times of quasinormal modes in ringdown gravitational waves with the Hilbert-Huang transform
• Seismic array measurements at Virgo's West End Building for the configuration of a Newtonian-noise cancellation system
• Exploring gravitational-wave detection and parameter inference using Deep Learning methods
• Probing the speed of gravity with LVK, LISA, and joint observations
• Gravitational waves carry information beyond effective spin parameters but it is hard to extract
• GWitchHunters: Machine Learning and citizen science to improve the performance of Gravitational Wave detector
• Detection and characterization of spin-orbit resonances in the advanced gravitational wave detectors era
• First results and future prospects for dual-harmonic searches for gravitational waves from spinning neutron stars
• GW150914: First search for the electromagnetic counterpart of a gravitational-wave event by the TOROS collaboration
• Systematic bias due to eccentricity in parameter estimation for merging binary neutron stars
• Wave effect of gravitational waves intersected with a microlens field: a new algorithm and supplementary study
• Improvements in Gravitational-Wave Sky Localization with Expanded Networks of Interferometers
• The reliability of the low-latency estimation of binary neutron star chirp mass
• Ordering the confusion: A study of the impact of lens models on gravitational-wave lensing detection capabilities
• Frequency space derivation of linear and non-linear memory gravitational wave signals from eccentric binary orbits
• Measurement of optical losses in a high-finesse 300 m filter cavity for broadband quantum noise reduction in gravitational-wave detectors
• The KAGRA underground environment and lessons for the Einstein Telescope
• Frequentist versus Bayesian analyses: Cross-correlation as an (approximate) sufficient statistic for LIGO-Virgo stochastic background searches
• High-accuracy simulations of highly spinning binary neutron star systems
• Search for continuous gravitational waves from ten H.E.S.S. sources using a hidden Markov model
• Mirror actuation design for the interferometer control of the KAGRA gravitational wave telescope
• General-Relativistic Hydrodynamics Simulation of a Neutron Star - Sub-Solar-Mass Black Hole Merger
• Generalized uncertainty principle in resonant detectors of gravitational waves
• Gravitational Waves from Black-Hole Encounters: Prospects for Ground- and Galaxy-Based Observatories
• Effect of orbital eccentricity on the dynamics of precessing compact binaries
• On the equal-mass limit of precessing black-hole binaries
• Inverse-chirp signals and spontaneous scalarisation with self-interacting potentials in stellar collapse
• Anisotropies in Scalar-Induced Gravitational-Wave Background from Inflaton-Curvaton Mixed Scenario with Sound Speed Resonance
• Converting the signal-recycling cavity into an unstable optomechanical filter to enhance the detection bandwidth of gravitational-wave detectors
• Using machine learning to parametrize postmerger signals from binary neutron stars
• Assessing and Mitigating the Impact of Glitches on Gravitational-Wave Parameter Estimation: a Model Agnostic Approach
• Synthetic FM triplet for AM-free precision laser stabilization and spectroscopy
• Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?
• Inferring host-galaxy properties of LIGO-Virgo-KAGRA's black holes
• Classification of the core-collapse supernova explosion mechanism with learned dictionaries
• Probing the Birth of Post-merger Millisecond Magnetars by X-ray and Gamma-ray Emission
• Localization of Binary Black-Hole Mergers with Known Inclination
• Constraining neutron star properties with a new equation of state insensitive approach
• Constraints on the merging binary neutron star mass distribution and equation of state based on the incidence of jets in the population
• Accuracy of the Post-Newtonian Approximation for Extreme-Mass Ratio Inspirals from Black-hole Perturbation Approach
• Rapid localization of gravitational wave sources from compact binary coalescences using deep learning
• Particle swarm optimization of the sensitivity of a cryogenic gravitational wave detector
• Hints of spin-orbit resonances in the binary black hole population
• Constraining the Neutron Star Radius with Joint Gravitational-Wave and Short Gamma-Ray Burst Observations of Neutron Star-Black Hole Coalescing Binaries
• Facilitating follow-up of LIGO-Virgo events using rapid sky localization
• Rapid parameter estimation for an all-sky continuous gravitational wave search using conditional varitational auto-encoders
• Tidal heating as a direct probe of strangeness inside neutron stars
• Post-Newtonian templates for gravitational waves from compact binary inspirals
• Probing the large scale structure using gravitational-wave observations of binary black holes
• Swift-XRT Follow-up of Gravitational Wave Triggers in the Second Advanced LIGO/Virgo Observing Run
• Observational prospects of self-interacting scalar superradiance with next-generation gravitational-wave detectors
• Faster search for long gravitational-wave transients: GPU implementation of the transient F-statistic
• Particle Swarm Optimization based search for gravitational waves from compact binary coalescences: performance improvements
• Understanding binary neutron star collisions with hypermodels
• Advancing Space-Based Gravitational Wave Astronomy: Rapid Parameter Estimation via Normalizing Flows
• Explodability fluctuations of massive stellar cores enable asymmetric compact object mergers such as GW190814
• The stepping-stone sampling algorithm for calculating the evidence of gravitational wave models
• Prospects for detecting transient quasi-monochromatic gravitational waves from glitching pulsars with current and future detectors
• Evolution of dwarf galaxies hosting GW150914-like events
• Weakly-Gravitating Objects in dynamical Chern-Simons gravity and Constraints with Gravity Probe B
• Biases in estimates of black hole kicks from the spin distribution of binary black holes
• Adding higher-order spherical harmonics in non-spinning eccentric binary black hole merger waveform models
• Counting on Short Gamma-Ray Bursts: Gravitational-Wave Constraints of Jet Geometry
• Constraint on Brans-Dicke theory from intermediate/extreme mass ratio inspirals
• Using Equation of State Constraints to Classify Low-Mass Compact Binary Mergers
• Template bank for spinning compact binary mergers in the second observation run of Advanced LIGO and the first observation run of Advanced Virgo
• The impact of selection biases on tests of general relativity with gravitational-wave inspirals
• Gravitational Wave Timing Array
• Upper limits on the Polarized Isotropic Stochastic Gravitational-Wave Background from Advanced LIGO-Virgo's First Three Observing Runs
• PyROQ: a Python-based Reduced Order Quadrature Building Code for Fast Gravitational Wave Inference
• Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits
• Arm locking performance with the new LISA design
• Waves from the Centre: Probing PBH and other Macroscopic Dark Matter with LISA
• Using Gray Sirens to Resolve the Hubble-Lemaître Tension
• An Isotropy Measurement with Gravitational Wave Observations
• Effective one body Hamiltonian in scalar-tensor gravity at third post-Newtonian order
• Pre-merger sky localization of gravitational waves from binary neutron star mergers using deep learning
• Searching for spin-2 ULDM with gravitational waves interferometers
• Generalised gravitational burst generation with Generative Adversarial Networks
• Numerical simulations of black hole-neutron star mergers in scalar-tensor gravity
• Quasinormal Modes for Dynamical Black Holes
• Inferring the Intermediate Mass Black Hole Number Density from Gravitational Wave Lensing Statistics
• Highly reflective low-noise etalon-based meta-mirror
• Investigating the effect of in-plane spin directions for Precessing BBH systems
• Predicting the properties of black holes merger remnants with Deep Neural Networks
• Calibration Uncertainty's Impact on Gravitational-Wave Observations
• Testing the Kerr nature of intermediate-mass and supermassive black hole binaries using spin-induced multipole moment measurements
• The Multi-mode Acoustic Gravitational Wave Experiment: MAGE
• Unveiling Microlensing Biases in Testing General Relativity with Gravitational Waves
• Probing neutron star structure via f-mode oscillations and damping in dynamical spacetime models
• Unified mapmaking for an anisotropic stochastic gravitational wave background
• Establishing the significance of continuous gravitational-wave detections from known pulsars
• Eccentricity signatures in LIGO-Virgo-KAGRA's BNS and NSBH binaries
• Investigation of magnetic noise in Advanced Virgo
• Virgo Detector Characterization and Data Quality: tools
• Reconstructing Gravitational Wave Core-Collapse Supernova Signals with Dynamic Time Warping
• Stochastic Gravitational Waves from Post-inflationary Structure Formation
• Gravitational Waves from Phase Transition in Minimal SUSY $U(1{)}_{B-L}$ Model
• Physical Models for the Astrophysical Population of Black Holes: Application to the Bump in the Mass Distribution of Gravitational Wave Sources
• Search for continuous gravitational waves from Fomalhaut b in the second Advanced LIGO observing run with a hidden Markov model
• Inferring neutron star properties with continuous gravitational waves
• Characterizing Astrophysical Binary Neutron Stars with Gravitational Waves
• Searching for anisotropic stochastic gravitational-wave backgrounds with constellations of space-based interferometers
• Numerical relativity higher order gravitational waveforms of eccentric, spinning, non-precessing binary black hole mergers
• Frequency planning for LISA
• Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds
• Establishing significance of gravitational-wave signals from a single observatory in the PyCBC offline search
• Huddle test measurement of a near Johnson noise limited geophone
• Rapid model comparison of equations of state from gravitational wave observation of binary neutron star coalescences
• Fundamental physics using the temporal gravitational wave background
• Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels
• On Improving the Performance of Glitch Classification for Gravitational Wave Detection by using Generative Adversarial Networks
• A tale of tails through generalized unitarity
• A classifier for gravitational-wave inspiral signals in non-ideal single-detector data
• Ancestral Black Holes of Binary Merger GW190521
• Identifying strongly lensed gravitational waves through their phase consistency
• Searching for Gamma-Ray counterparts to Gravitational Waves from merging binary neutron stars with the Cherenkov Telescope Array
• Real-Time Detection of Unmodelled Gravitational-Wave Transients Using Convolutional Neural Networks
• Radiation Reaction for Non-Spinning Bodies at 4.5PN in the Effective Field Theory Approach
• Optimized Search for a Binary Black Hole Merger Population in LIGO-Virgo O3 Data
• Correlated 0.01Hz-40Hz seismic and Newtonian noise and its impact on future gravitational-wave detectors
• Self-consistent MHD simulation of jet launching in a neutron star - white dwarf merger
• GW150914 peak frequency: a novel consistency test of strong-field General Relativity
• Gravitational-Wave Searches for Cosmic String Cusps in Einstein Telescope Data using Deep Learning
• Efficient Reduced Order Quadrature Construction Algorithms for Fast Gravitational Wave Inference
• Accelerated binary black holes in globular clusters: forecasts and detectability in the era of space-based gravitational-wave detectors
• LIGO-Virgo-KAGRA's Oldest Black Holes: Probing star formation at cosmic noon with GWTC-3
• Analyzing black-hole ringdowns II: data conditioning
• Compact Binary Coalescences in Dense Gaseous Environments Can Pose as ones in Vacuum
• Eccentric first post-Newtonian waveforms for compact binaries in frequency domain with Hansen coefficients
• GRB 211211A-like Events and How Gravitational Waves May Tell Their Origins
• Constraining Horndeski theory with gravitational waves from coalescing binaries
• Rapid population synthesis of black-hole high-mass X-ray binaries: implications for binary stellar evolution
• Detection of high-frequency gravitational waves using high-energy pulsed lasers
• Glitch subtraction from gravitational wave data using adaptive spline fitting
• Self-Interacting Gravitational Atoms in the Strong-Gravity Regime
• Post-merger chirps from binary black holes as probes of the final black-hole horizon
• Accretion-modified stellar-mass black hole distribution and milli-Hz gravitational wave backgrounds from galaxy centre
• Needle in a Bayes Stack: a Hierarchical Bayesian Method for Constraining the Neutron Star Equation of State with an Ensemble of Binary Neutron Star Post-merger Remnants
• A Robust Test of the Existence of Primordial Black Holes in Galactic Dark Matter Halos
• Convolutional neural network for gravitational-wave early alert: Going down in frequency
• Resampling to accelerate cross-correlation searches for continuous gravitational waves from binary systems
• D-term inflation in braneworld models: Consistency with cosmic-string bounds and early-time Hubble tension resolving models
• Performance of Particle Swarm Optimization on the fully-coherent all-sky search for gravitational waves from compact binary coalescences
• Constraining the Gravitational-Wave Afterglow From a Binary Neutron Star Coalescence
• A lower limit for Newtonian-noise models of the Einstein Telescope
• Localization of Compact Binary Sources with Second Generation Gravitational-wave Interferometer Networks
• Future Gravitational Wave Detectors Based on Atom Interferometry
• Realistic observing scenarios for the next decade of early warning detection of binary neutron stars
• Timing-residual power spectrum of a polarized stochastic gravitational-wave background in pulsar-timing-array observation
• Kilonova and Optical Afterglow from Binary Neutron Star Mergers. II. Optimal Search Strategy for Serendipitous Observations and Target-of-opportunity Observations of Gravitational-wave Triggers
• Gravitational Multipole Renormalization
• Stochastic gravitational-wave background searches and constraints on neutron-star ellipticity
• Application of the Hilbert-Huang transform for analyzing standing-accretion-shock-instability induced gravitational waves in a core-collapse supernova
• Stability of the protoneutron stars toward black hole formation
• Search for Black Hole Merger Families
• Extending the frequency reach of pulsar timing array based gravitational wave search without high cadence observations
• LIGO as a probe of Dark Sectors
• Speed of sound in dense matter and two families of compact stars
• Deep Learning Model on Gravitational Waveforms in Merging and Ringdown Phases of Binary Black Hole Coalescences
• Lensing magnification: gravitational waves from coalescing stellar-mass binary black holes
• Optimising the choice of analysis method for all-sky searches for continuous gravitational waves with Einstein@Home
• Exact one-loop false vacuum decay rate
• "Stairway to Heaven" -- Spectroscopy of Particle Couplings with Gravitational Waves
• Search for Long-duration Gravitational-wave Signals Associated with Magnetar Giant Flares
• The Palomar Transient Factory Sky2Night programme
• Continuous Gravitational Waves: A New Window to Look for Heavy Non-annihilating Dark Matter
• Mergers of Maximally Charged Primordial Black Holes
• Spin Doctors: How to diagnose a hierarchical merger origin
• Ternary Quarter Wavelength Coatings for Gravitational Wave Detector Mirrors: Design Optimization via Exhaustive Search
• Forecasts on interacting dark energy with standard sirens
• Detecting non-Gaussian gravitational wave backgrounds: a unified framework
• KilonovaNet: Surrogate Models of Kilonova Spectra with Conditional Variational Autoencoders
• The interplay of astrophysics and nuclear physics in determining the properties of neutron stars
• An arm length stabilization system for KAGRA and future gravitational-wave detectors
• Impact of ringdown higher-order modes on black-hole mergers in dense environments: the scalar field case, detectability and parameter biases
• Formation of Merging Stellar-Mass Black Hole Binaries by Gravitational Wave Emission in Active Galactic Nucleus Disks
• Post-inflationary thermal histories and the refractive index of relic gravitons
• Dynamic Scheduling: Target of Opportunity Observations of Gravitational Wave Events
• Detectability of continuous gravitational waves from isolated neutron stars in the Milky Way: the population synthesis approach
• The lure of sirens: joint distance and velocity measurements with third generation detectors
• Active platform stabilisation with a 6D seismometer
• Seismic Cross-coupling Noise in Torsion Pendulums
• Matter Effects on LIGO/Virgo Searches for Gravitational Waves from Merging Neutron Stars
• Towards mitigating the effect of sine-Gaussian noise transients on searches for gravitational waves from compact binary coalescences
• Using supervised learning algorithms as a follow-up method in the search of gravitational waves from core-collapse supernovae
• Binary Black Hole Merger Rates Inferred from Luminosity Function of Ultra-Luminous X-ray Sources
• Enhanced primordial gravitational waves from a stiff post-inflationary era due to an oscillating inflaton
• Characterization of Laser Systems at 1550 nm Wavelength for Future Gravitational Wave Detectors
• Concurrent estimation of noise and compact-binary signal parameters in gravitational-wave data
• Backward Population Synthesis: Mapping the Evolutionary History of Gravitational-Wave Progenitors
• Prospects of joint detections of neutron star mergers and short-GRBs with Gaussian structured jets
• An implementation of Galactic white dwarf binary data analysis for MLDC-3.1
• All-sky radiometer for narrowband gravitational waves using folded data
• Dark Black Holes in the Mass Gap
• Optimal phase sensitivity of an unbalanced Mach-Zehnder interferometer
• The astrophysical odds of GW151216
• Adding equatorial-asymmetric effects for spin-precessing binaries into the SEOBNRv5PHM waveform model
• Strategies for the Follow-up of Gravitational Wave Transients with the Cherenkov Telescope Array
• Bayesian search for gravitational wave bursts in pulsar timing array data
• Detecting Fundamental Vector Fields with LISA
• Effects of orbital precession on hyperbolic encounters
• Rapidly rotating neutron star progenitors
• Enhancing the sensitivity of transient gravitational wave searches with Gaussian Mixture Models
• Convolutional neural network search for long-duration transient gravitational waves from glitching pulsars
• Photo-Thermal Transfer Function of Dielectric Mirrors for Precision Measurements
• Swift sky localization of gravitational waves using deep learning seeded importance sampling
• Phenomenological relationship between eccentric and quasi-circular orbital binary black hole waveform
• Incorporation of model accuracy in gravitational wave Bayesian inference
• The Linear Regime of Tachyonic Preheating
• Magnetic coupling to the Advanced Virgo payloads and its impact on the low frequency sensitivity
• Dilated convolutional neural network for detecting extreme-mass-ratio inspirals
• Hierarchical Bayesian method for detecting continuous gravitational waves from an ensemble of pulsars
• Detectability of Primordial Black Hole Binaries at High Redshift
• Parametrized spin-precessing inspiral-merger-ringdown waveform model for tests of general relativity
• Generalized Uncertainty Principle mimicking dynamical Dark Energy: matter perturbations and gravitational wave data analysis
• Multimessenger astronomy with a kHz-band gravitational-wave observatory
• On GW170817 and the Galactic Binary Neutron Star Population
• Angular Resolution of the Search for Anisotropic Stochastic Gravitational-Wave Background with Terrestrial Gravitational-Wave Detectors
• Gravitational waveforms of binary neutron star inspirals using post-Newtonian tidal splicing
• A stochastic search for intermittent gravitational-wave backgrounds
• Modeling Mergers of Known Galactic Systems of Binary Neutron Stars
• Breaking bad degeneracies with Love relations: Improving gravitational-wave measurements through universal relations
• Multi-messenger Gravitational Lensing
• Hubble constant and nuclear equation of state from kilonova spectro-photometric light curves
• Targeted search for the stochastic gravitational-wave background from the galactic millisecond pulsar population
• Gravitational Waves from Accreting Neutron Stars undergoing Common-Envelope Inspiral
• Analytic thin wall false vacuum decay rate
• GWSim: Python package for creating mock GW samples for different astrophysical populations and cosmological models of binary black holes
• Consistent eccentricities for gravitational wave astronomy: Resolving discrepancies between astrophysical simulations and waveform models
• Inspiral-Merger-Ringdown Consistency Tests with Higher Modes on Gravitational Signals from the Second Observing Run of LIGO and Virgo
• No evidence that the binary black hole mass distribution evolves with redshift
• Supermassive Binary Black Hole Evolution can be traced by a small SKA Pulsar Timing Array
• Signal Space in the Triangular Network of Einstein Telescope
• High bandwidth laser-frequency-locking for wideband noise suppression
• Observable Gravitational Waves from Hyperkination in Palatini Gravity and Beyond
• Novel directed search strategy to detect continuous gravitational waves from neutron stars in low- and high-eccentricity binary systems
• Defining eccentricity for spin-precessing binaries
• Enabling multi-messenger astronomy with continuous gravitational waves: early warning and sky localization of binary neutron stars in Einstein Telescope
• Gravitational-wave follow-up with CTA after the detection of GRBs in the TeV energy domain
• Inferring Parameters of GW170502: The Loudest Intermediate-mass Black Hole Trigger in LIGO's O1/O2 data
• Analysis of GWTC-3 with fully precessing numerical relativity surrogate models
• Opportunities and limits of lunar gravitational-wave detection
• Linear vs. nonlinear modeling of black hole ringdowns
• Calibrating the cosmic distance ladder using gravitational-wave observations
• Possible binary neutron star merger history of the primary of GW230529
• Scalarization of isolated black holes in scalar Gauss-Bonnet theory in the fixing-the-equations approach
• A waveform model for the missing quadrupole mode from black hole coalescence: memory effect and ringdown of the $(\ell =2,m=0)$ spherical harmonic
• A geometric template bank for the detection of spinning low-mass compact binaries with moderate orbital eccentricity
• Searching for cosmological stochastic backgrounds by notching out resolvable compact binary foregrounds with next-generation gravitational-wave detectors
• A Challenge to Identify an Optical Counterpart of the Gravitational Wave Event GW151226 with Hyper Suprime-Cam
• Implications of the Quantum Noise Target for the Einstein Telescope Infrastructure Design
• Primordial Gravitational Waves Assisted by Cosmological Scalar Perturbations
• Mimicking Mergers: Mistaking Black Hole Captures as Mergers
• Localization of binary neutron star mergers with a single Cosmic Explorer
• A six degree-of-freedom fused silica seismometer: Design and tests of a metal prototype
• Applying the Viterbi Algorithm to Planetary-Mass Black Hole Searches
• Hierarchical approach to matched filtering using a reduced basis
• Identifying glitches near gravitational-wave signals from compact binary coalescences using the Q-transform
• Piezo-deformable Mirrors for Active Mode Matching in Advanced LIGO
• Observational Signatures of Highly Magnified Gravitational Waves from Compact Binary Coalescence
• Deep Learning-based Search for Microlensing Signature from Binary Black Hole Events in GWTC-1 and -2
• What if GW190425 did not produce a black hole promptly?
• Silicon emissivity as a function of temperature
• Targeted modeling of GW150914's binary black hole source with dart_board
• Gravitational wave memory of compact binary coalescence in the presence of matter effects
• Nonlinear dynamics of oscillating neutron stars in scalar-tensor gravity
• First eccentric inspiral-merger-ringdown analysis of neutron star-black hole mergers
• Late-time tails in nonlinear evolutions of merging black holes
• Merging black holes with Cauchy-characteristic matching: Computation of late-time tails
• Measurement of the Cross-Correlation Angular Power Spectrum Between the Stochastic Gravitational Wave Background and Galaxy Over-Density
• Multi-messenger astronomy of gravitational-wave sources with flexible wide-area radio transient surveys
• Model-independent estimation of the cosmography parameters using cosmic chronometers
• Assessing gravitational-wave binary black hole candidates with Bayesian odds
• Enhancing phase sensitivity in Mach-Zehnder interferometer with various detection schemes using SU(1,1) coherent states
• Dynamical quasinormal mode excitation
• Observable Primordial Gravitational Waves from Non-minimally Coupled $R^2$ Palatini Modified Gravity
• Bayesian modelling of scattered light in the LIGO interferometers
• Footprints of population III stars in the gravitational-wave background
• Matrix Heater in the Gravitational Wave Observatory GEO 600
• Tackling excess noise from bilinear and nonlinear couplings in gravitational-wave interferometers
• LISA Telescope: Phase noise due to pointing jitter
• Gravitational-wave parameter inference with the Newman-Penrose scalar ${\psi }_4$
• Evidence of the pair instability gap from black hole masses
• Search for gravitational waves emitted from SN 2023ixf
• Improved early warning of compact binary mergers using higher modes of gravitational radiation: A population study
• Nonchaotic evolution of triangular configuration due to gravitational radiation reaction in the three-body problem
• Application of the third RIT binary black hole simulations catalog to parameter estimation of gravitational waves signals from the LIGO-Virgo O1/O2 observational runs
• Prompt sky localization of compact binary sources using a meshfree approximation
• Searching for MHz Gravitational Waves from Harmonic Sources
• Relativistic correction to the r-mode frequency in light of multi-messenger constraints
• Detection of LIGO-Virgo binary black holes in the pair-instability mass gap
• Neutron stars formation and Core Collapse Supernovae
• Measuring neutron-star distances and properties with gravitational-wave parallax
• Observing the dark sector
• Enhancing the significance of gravitational wave bursts through signal classification
• Measurement of the Newtonian Constant of Gravitation $G$ by Precision Displacement Sensors
• Frequency-dependent squeezing for gravitational-wave detection through quantum teleportation
• Establishing connection between neutron star properties and nuclear matter parameters through a comprehensive multivariate analysis
• Untangling PBH overproduction in $w$-SIGWs generated by Pulsar Timing Arrays for MST-EFT of single field inflation
• Calibrating gravitational-wave detectors with GW170817
• Universal phenomenological relations between spherical harmonic modes in non-precessing eccentric binary black hole merger waveforms
• Feasibility of near-unstable cavities for future gravitational wave detectors
• How would GW150914 look with future GW detector networks?
• Searching for high-frequency gravitational waves by ground high field magnetic resonant sweepings
• Constraining the Gravitational-Wave Spectrum from Cosmological First-Order Phase Transitions Using Data from LIGO-Virgo First Three Observing Runs
• Self-Gravity Effects of Ultralight Boson Clouds Formed by Black Hole Superradiance
• Search for Gravitational Waves from Scorpius X-1 in LIGO O3 Data With Corrected Orbital Ephemeris
• Quasinormal modes and echo effect of cylindrical anti-de Sitter black hole spacetime with a thin shell
• Characterization of low-significance gravitational-wave compact binary sources
• Prediction of crystallized phases of amorphous Ta${}_2$O${}_5$-based mixed oxide thin films using density functional theory calculations
• Measuring Spin of the Remnant Black Hole from Maximum Amplitude
• Technologies for the ELGAR large scale atom interferometer array
• Observational limits on the rate of radiation-driven binary black hole capture events
• Nonlinear gravitational-wave memory from cusps and kinks on cosmic strings
• Detectability of the cross-correlation between CMB lensing and stochastic GW background from compact object mergers
• Constraining binary mergers in AGN disks using the non-observation of lensed gravitational waves
• Heavy-tailed likelihoods for robustness against data outliers: Applications to the analysis of gravitational wave data
• One to many: comparing single gravitational-wave events to astrophysical populations
• Autoencoder-driven Spiral Representation Learning for Gravitational Wave Surrogate Modelling
• Experimental demonstrations of alignment and mode matching in optical cavities with higher-order Hermite-Gauss modes
• Waterfall stiff period can generate observable primordial gravitational waves
• HEALPix Alchemy: Fast All-Sky Geometry and Image Arithmetic in a Relational Database for Multimessenger Astronomy Brokers
• Gravitational waves from neutron-star mountains
• Ranking Candidate Signals with Machine Learning in Low-Latency Search for Gravitational-Waves from Compact Binary Mergers
• Probing resonant excitations in exotic compact objects via gravitational waves
• Effect of double spin-precession and higher harmonics on spin-induced quadrupole moment measurements
• Ground motion prediction at gravitational wave observatories using archival seismic data
• Template Lattices for a Cross-Correlation Search for Gravitational Waves from Scorpius X-1
• On Detecting Stellar Binary Black Holes via the LISA-Taiji Network
• Rotational-tidal phasing of the binary neutron star waveform
• Systematic errors due to quasi-universal relations in binary neutron stars and their correction for unbiased model selection
• Towards observing the neutron star collapse with gravitational wave detectors
• Detecting compact galactic binaries using a hybrid swarm-based algorithm
• Power coupling losses for misaligned and mode-mismatched higher-order Hermite-Gauss modes
• Bilinear noise subtraction at the GEO 600 observatory
• Tracking continuous gravitational waves from a neutron star at once and twice the spin frequency with a hidden Markov model
• Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes
• Calibrating signal-to-noise ratio detection thresholds using gravitational-wave catalogs
• Neutron star mass in dark matter clumps
• Indication for a compact object next to a LIGO-Virgo binary black hole merger
• The Zadko Telescope: Exploring the transient Universe
• Compactness peaks: An astrophysical interpretation of the mass distribution of merging binary black holes
• Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
• The Quantum Memory Matrix: A Unified Framework for the Black Hole Information Paradox
• Unveiling the Nature of Gravitational-Wave Emission in Core-collapse Supernovae with Perturbative Analysis
• Transition of EMRIs through resonance: corrections to higher order in the on-resonance flux modification
• Incorporating information from LIGO data quality streams into the PyCBC search for gravitational waves
• Boosting the sensitivity of high frequency gravitational wave detectors by PT-symmetry
• Merger rate density of stellar-mass binary black holes from young massive clusters, open clusters, and isolated binaries: comparisons with LIGO-Virgo-KAGRA results
• Long-duration transient, gravitational-wave search pipeline
• On the gauge dependence of scalar induced secondary gravitational waves during radiation and matter domination eras
• Inspirals into a charged black hole
• Observational implications of lowering the LIGO-Virgo alert threshold
• Inconsistent black hole kick estimates from gravitational-wave models
• Search setup for long-duration transient gravitational waves from glitching pulsars during LIGO-Virgo third observing run
• Search for Advanced LIGO Single Interferometer Compact Binary Coalescence Signals in Coincidence with Gamma-Ray Events in Fermi-GBM
• The False Alarms induced by Gaussian Noise in Gravitational Wave Detectors
• Did Goryachev et al. detect megahertz gravitational waves?
• Intermediate-mass black hole binary parameter estimation with next-generation ground-based detector networks
• Constraining the delay time distribution of compact binary objects from the stochastic gravitational wave background searches
• Impact of combinations of time-delay interferometry channels on stochastic gravitational wave background detection
• Efficient fully precessing gravitational waveforms for binaries with neutron stars
• ArchEnemy: Removing scattered-light glitches from gravitational wave data
• Probing the pulsar explanation of the Galactic-Center GeV excess using continuous gravitational-wave searches
• All-sky, narrowband, gravitational-wave radiometry with folded data
• Gravitational wave peak luminosity model for precessing binary black holes
• Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries
• Time-frequency track distance for comparing continuous gravitational wave signals
• Thermal charge carrier driven noise in transmissive semiconductor optics
• Precision Ephemerides for Gravitational-wave Searches -- IV: Corrected and refined ephemeris for Scorpius X-1
• A robust cosmic standard ruler from the cross-correlations of galaxies and dark sirens
• Constraining the AGN formation channel for detected black hole binary mergers up to z=1.5 with the Quaia catalogue
• Optical and mechanical properties of ion-beam-sputtered MgF${}_2$ thin films for gravitational-wave interferometers
• Multi-messenger observations of core-collapse supernovae: Exploiting the standing accretion shock instability
• Direct mapping of tidal deformability to the iso-scalar and iso-vector nuclear matter parameters
• Gravitational wave detection from OJ 287 via a pulsar timing array
• The failure of the Fisher Matrix when including tidal terms: Considering construction of template banks of tidally deformed binary neutron stars
• Recipes for computing radiation from a Kerr black hole using a generalized Sasaki-Nakamura formalism: Homogeneous solutions
• Supporting High-Performance and High-Throughput Computing for Experimental Science
• Microlensing bias on the detection of strong lensing gravitational wave
• Subtraction of the confusion foreground and parameter uncertainty of resolvable galactic binaries on the networks of space-based gravitational-wave detectors
• Web application for galaxy-targeted follow-up of electromagnetic counterparts to gravitational wave sources
• The Impact of Black Hole Scaling Relation Assumptions on the Mass Density of Black Holes
• Thermal modelling of Advanced LIGO test masses
• Bayesian inference for binary neutron star inspirals using a Hamiltonian Monte Carlo Algorithm
• Gravitational-wave Observations Suggest Most Black Hole Mergers Form in Triples
• New methods to assess and improve LIGO detector duty cycle
• Potential biases and prospects for the Hubble constant estimation via electromagnetic and gravitational-wave joint analyses
• Astrophysical signal consistency test adapted for gravitational-wave transient searches
• Numerical convergence of model Cauchy-characteristic extraction and matching
• Posterior samples of the parameters of binary black holes from Advanced LIGO, Virgo's second observing run
• Suspension-thermal noise in spring-antispring systems for future gravitational-wave detectors
• Gravitational-wave imprints of non-convex dynamics in binary neutron star mergers
• Rapid gravitational wave parameter estimation with a single spin: Systematic uncertainties in parameter estimation with the SpinTaylorF2 approximation
• Localization of gravitational waves using machine learning
• Implications for Cosmic Domain Walls from LIGO-Virgo First Three Observing Runs
• Neural network time-series classifiers for gravitational-wave searches in single-detector periods
• Chasing 5-sigma: Prospects for searches for long-duration gravitational-waves without time slides
• Impact of unmodeled eccentricity on the tidal deformability measurement and implications for gravitational wave physics inference
• LOFAR 144-MHz follow-up observations of GW170817
• An observational upper limit on the rate of gamma-ray bursts with neutron star-black hole merger progenitors
• A stochastic template bank for gravitational wave searches for precessing neutron-star--black-hole coalescence events
• What Determines the Maximum Mass of AGN-assisted Black Hole Mergers?
• A method for the experimental measurement of bulk and shear loss angles in amorphous thin films
• Templated Anisotropic Analyses of the LISA Galactic Foreground
• Rapid inference and comparison of gravitational-wave population models with neural variational posteriors
• Constraining the Break of Spatial Diffeomorphism Invariance with Planck Data
• Mitigating the binary viewing angle bias for standard sirens
• Gravitational wave emission from dynamical stellar interactions
• Accounting for numerical-relativity calibration uncertainty in gravitational-wave modeling and inference
• Constraining hierarchical mergers of binary black holes detectable with LIGO-Virgo
• Macroscopic quantum entanglement between an optomechanical cavity and a continuous field in presence of non-Markovian noise
• Rapid localization of gravitational wave hosts with FIGARO
• Exploring a search for long-duration transient gravitational waves associated with magnetar bursts
• Information Retrieval and Recommendation System for Astronomical Observatories
• Quasinormal Modes in Modified Gravity using Physics-Informed Neural Networks
• Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review
• Optimal Optical Search Strategy for Finding Transient in Large Sky Error Region Under Realistic Constraints
• GWDALI: A Fisher-matrix based software for gravitational wave parameter-estimation beyond Gaussian approximation
• Comparing hierarchical black hole mergers in star clusters and active galactic nuclei
• Formation of GW230529 from Isolated Binary Evolution
• Will Gravitational Wave Sirens Determine the Hubble Constant?
• Subdominant Modes of Scalar Superradiant Instability and Gravitational Wave Beats
• Possible confirmation of the existence of ergoregion by the Kerr quasinormal mode in gravitational waves from Pop III massive black hole binary
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• Boltzmann equations for astrophysical Stochastic Gravitational Wave Backgrounds scattering off of massive objects
• Mode matching error signals using radio-frequency beam shape modulation
• Be careful in multi-messenger inference of the Hubble constant: A path forward for robust inference
• Structure and Skewness of the Effective Inspiral Spin Distribution of Binary Black Hole Mergers
• Robust constraints on tensor perturbations from cosmological data: a comparative analysis from Bayesian and frequentist perspectives
• Parametrized tests of general relativity using eccentric compact binaries
• Possibility of primordial black holes as the source of gravitational wave events in the advanced LIGO detector
• Formalism for power spectral density estimation for non-identical and correlated noise using the null channel in Einstein Telescope
• Comparative study of 1D and 2D convolutional neural network models with attribution analysis for gravitational wave detection from compact binary coalescences
• Towards a robust and reliable deep learning approach for detection of compact binary mergers in gravitational wave data
• On the Role of Muons in Binary Neutron Star Mergers: First Simulations
• Stochastic gravitational wave background: birth from string-wall death
• Measurement of the Stray Light in the Advanced Virgo Input Mode Cleaner Cavity using an instrumented baffle
• Validating continuous gravitational-wave candidates from a semicoherent search using Doppler modulation and an effective point spread function
• Effects of mixing and annealing on the optical and mechanical properties of TiO${}_2$:Ta${}_2$O${}_5$ amorphous coatings
• An independent search of gravitational waves in the first observation run of advanced LIGO using cross-correlation
• Measuring violations of General Relativity from single gravitational wave detection by non-spinning binary systems: higher-order asymptotic analysis
• Improvement of the parameter measurement accuracy by the third-generation gravitational wave detector Einstein Telescope
• Visualizing convolutional neural network for classifying gravitational waves from core-collapse supernovae
• Parameter Estimation for Tests of General Relativity with the Astrophysical Stochastic Gravitational Wave Background
• J-GEM optical and near-infrared follow-up of gravitational wave events during LIGO's and Virgo's third observing run
• Feasibility study of beam-expanding telescopes in the interferometer arms for the Einstein Telescope
• Search for continuous gravitational wave signals from luminous dark photon superradiance clouds with LVK O3 observations
• The SPIIR online coherent pipeline to search for gravitational waves from compact binary coalescences
• Bounds on tidal charges from gravitational-wave ringdown observations
• A hybrid silicon-sapphire cryogenic Fabry-Perot cavity using hydroxide catalysis bonding
• Parameter estimation of microlensed gravitational waves with Conditional Variational Autoencoders
• Stochastic waveform estimation at the fundamental quantum limit
• Prospects of calibrating afterglow modeling of short GRBs with gravitational wave inclination angle measurements and resolving the Hubble tension with a GW-GRB association event
• Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
• Jointly setting upper limits on multiple components of an anisotropic stochastic gravitational-wave background
• MOCCA-SURVEY Database -- I. Tidal disruption events of white dwarfs in globular clusters and young massive clusters
• A Search for IceCube sub-TeV Neutrinos Correlated with Gravitational-Wave Events Detected By LIGO/Virgo
• Real modes and null memory contributions in effective-one-body models
• Constrains of the axion-like particle from black hole spin superradiance
• Improved parametrized test of general relativity using the IMRPhenomX waveform family: Including higher harmonics and precession
• Optimizing post-Newtonian parameters and fixing the BMS frame for numerical-relativity waveform hybridizations
• Gravitational-wave event rates as a new probe for dark matter microphysics
• Central X-ray point-sources found to be abundant in low-mass, late-type galaxies predicted to contain an intermediate-mass black hole
• Search for Coincident Gravitational-wave and Fast Radio Burst Events from 4-OGC and the First CHIME/FRB Catalog
• Noise in the LIGO Livingston Gravitational Wave Observatory due to Trains
• - Gravitational Waves - A Review on the Conceptual Foundations of Gravitational Radiation
• Silk Damping in Scalar-Induced Gravitational Waves: A Novel Probe for New Physics
• The imprint of superradiance on hierarchical black hole mergers
• Kilonova constraints for the LIGO/Virgo/KAGRA neutron star merger candidate S250206dm: GW-MMADS observations
• Seismic Background Limitation of Lunar Gravitational-wave Detectors
• Fully general relativistic simulations of rapidly rotating quark stars: Oscillation modes and universal relations
• Host galaxy identification for binary black hole mergers with long baseline gravitational wave detectors
• Training Process of Unsupervised Learning Architecture for Gravity Spy Dataset
• A Standard Siren Cosmological Measurement from the Potential GW190521 Electromagnetic Counterpart ZTF19abanrhr
• Cosmic Cartography: Bayesian reconstruction of the galaxy density informed by large-scale structure
• Multi-messenger Emission from Tidal Waves in Neutron Star Oceans
• Towards a Precision Measurement of Binary Black Holes Formation Channels Using Gravitational Waves and Emission Lines
• Gravitational lensing of gravitational waves: prospects for probing intermediate-mass black holes in galaxy lenses with global minima image
• Source localizations with the network of space-based gravitational wave detectors
• Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning
• Impact of anti-symmetric contributions to signal multipoles in the measurement of black-hole spins
• Parameter estimation using a complete signal and inspiral templates for low mass binary black holes with Advanced LIGO sensitivity
• Bayesian Reconstruction of Gravitational-wave Signals from Binary Black Holes with Nonzero Eccentricities
• Application of a Zero-latency Whitening Filter to Compact Binary Coalescence Gravitational-wave Searches
• Gravitational waves from axions annihilation through quantum field theory
• Prospects for measuring off-axis spins of binary black holes with Plus-era gravitational-wave detectors
• Reduction of quantum noise using the quantum locking with an optical spring for gravitational wave detectors
• Nondegenerate internal squeezing: an all-optical, loss-resistant quantum technique for gravitational-wave detection
• Echoes of axial gravitational perturbations in stars of uniform density
• Testing the nature of GW200105 by probing the frequency evolution of eccentricity
• $2\cdot 10^{-13}$ fractional laser frequency stability with a 7-cm unequal-arm Mach-Zehnder interferometer
• Mind the step: On the frequency-domain analysis of gravitational-wave memory waveforms
• Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars
• Do both black holes spin in merging binaries? Evidence from GWTC-4 and astrophysical implications
• A Coincidence Null Test for Poisson-Distributed Events
• Method to detect gravitational waves from an ensemble of known pulsars
• Early warning of precessing compact binary merger with third-generation gravitational-wave detectors
• Reexamining Evidence of a Pair-Instability Mass Gap in the Binary Black Hole Population
• Eclipses of continuous gravitational waves as a probe of stellar structure
• Kerr-Enhanced Optical Spring
• Nonorthogonal wavelet transformation for reconstructing gravitational wave signals
• Scalar Tops and Perturbed Quadrupoles: Probing Fundamental Physics with Spin-Precessing Binaries
• Scalable data-analysis framework for long-duration gravitational waves from compact binaries using short Fourier transforms
• Joint analysis of gravitational-wave and electromagnetic data of mergers: breaking an afterglow model degeneracy in GW170817 and in future events
• Search for ultralight dark matter with a frequency adjustable diamagnetic levitated sensor
• Optimal Sensor Fusion Method for Active Vibration Isolation Systems in Ground-Based Gravitational-Wave Detectors
• The detection of quasinormal mode with $a/M\sim 0.95$ would prove a sphere $99\%$ soaking in the ergoregion of the Kerr space-time
• The steep redshift evolution of the hierarchical binary black hole merger rate may cause the $z$-${\chi }_{\mathrm{eff}}$ correlation
• Parameter Estimation with Nonstationary Noise in Gravitational-wave Data
• Detecting Baryon Acoustic Oscillations with third generation gravitational wave observatories
• Nuclear physics with gravitational waves from neutron stars disrupted by black holes
• Prospects for the inference of inertial modes from hypermassive neutron stars with future gravitational-wave detectors
• Coherent coupling completes an unambiguous optomechanical classification framework
• Distinguishing a stochastic gravitational-wave signal from correlated noise with joint parameter estimation: Fisher analysis for ground-based detectors
• Method for detecting highly-eccentric binaries with a gravitational wave burst search
• Hunting Gravitational Waves with Multi-Messenger Counterparts: Australia's Role
• Premerger localization of intermediate mass binary black holes with LISA and prospects of joint observations with Athena and LSST
• A Mid-Thirties Crisis: Dissecting the Properties of Gravitational Wave Sources Near the 35 Solar Mass Peak
• Missed opportunities: GRB 211211A and the case for continual gravitational-wave coverage with a single observatory
• Bayesian parameter estimation for targeted anisotropic gravitational-wave background
• Can a binary neutron star merger in the vicinity of a supermassive black hole enable a detection of a post-merger gravitational wave signal?
• Search for continuous gravitational waves from PSR J0437$-$4715 with a hidden Markov model in O3 LIGO data
• Detectability of strongly lensed gravitational waves using model-independent image parameters
• A convolutional neural network to distinguish glitches from minute-long gravitational wave transients
• Dictionary learning: a novel approach to detecting binary black holes in the presence of Galactic noise with LISA
• Stellar Interferometry for Gravitational Waves
• No evidence for a dip in the binary black hole mass spectrum
• An interference-based method for the detection of strongly lensed gravitational waves
• Swift Multiwavelength Follow-up of LVC S200224ca and the Implications for Binary Black Hole Mergers
• Angular power spectra of anisotropic stochastic gravitational wave background: developing statistical methods and analyzing data from ground-based detectors
• The Critical Role of LIGO-India in the Era of Next-Generation Observatories
• Enhancing gravitational-wave burst detection confidence in expanded detector networks with the BayesWave pipeline
• Matched-filter study and energy budget suggest no detectable gravitational-wave 'extended emission' from GW170817
• Quantum Squeezing Schemes for Heterodyne Readout
• Detection of gravitational wave mixed polarization with single space-based detectors
• Constraints on Inflation with Null Energy Condition Violation from Advanced LIGO and Advanced Virgo's First Three Observing Runs
• Computational Techniques for Parameter Estimation of Gravitational Wave Signals
• What is the nature of GW230529? An exploration of the gravitational lensing hypothesis
• Implications of Fermionic Dark Matter Interactions on Anisotropic Neutron Stars
• Estimation of the gravitational wave polarizations from a non template search
• Effects of mirror birefringence and its fluctuations to laser interferometric gravitational wave detectors
• Development of ion-beam sputtered silicon nitride thin films for low-noise mirror coatings of gravitational-wave detectors
• A Stochastic Gravitational Wave Background in LISA from Unresolved White Dwarf Binaries in the Large Magellanic Cloud
• Quantum coherence of relic gravitons and Hanbury Brown-Twiss interferometry
• How to search for multiple messengers -- a general framework beyond two messengers
• Template bank to search for exotic gravitational wave signals from astrophysical compact binaries
• Determining the Hubble Constant with AGN-assisted Black Hole Mergers
• Numerically modeling Brownian thermal noise in amorphous and crystalline thin coatings
• A neural network emulator of the Advanced LIGO and Advanced Virgo selection function
• Accelerated detection of the binary neutron star gravitational-wave background
• Efficient Stochastic Template Bank using Inner Product Inequalities
• Testing the robustness of simulation-based gravitational-wave population inference
• A time domain experiment with Swift: monitoring of seven nearby galaxies
• Spline Based Search Method For Unmodeled Transient Gravitational Wave Chirps
• Impact of higher harmonics of gravitational radiation on the population inference of binary black holes
• Note on Accuracy of the Post-Newtonian Approximation for Extreme-Mass Ratio Inspirals: Retrograde Orbits
• Bayesian real-time classification of multi-messenger electromagnetic and gravitational-wave observations
• A model-independent tripartite test of cosmic distance relations
• Pinpointing coalescing binary neutron star sources with the IGWN, including LIGO-Aundha
• Measurements of Optical Scatter Versus Annealing Temperature for Amorphous Ta2O5 and TiO2:Ta2O5 Thin Films
• Negative non-Gaussianity as a salvager for PBHs with PTAs in bounce
• Particle production during Inflation with a non-minimally coupled spectator scalar field
• $\mu$-GLANCE: A Novel Technique to Detect Chromatically and Achromatically Lensed Gravitational Wave Signals
• Waveform systematics in identifying strongly gravitationally lensed gravitational waves: Posterior overlap method
• Misalignment and mode mismatch error signals for higher-order Hermite-Gauss modes from two sensing schemes
• A Unified $p_{\mathrm{astro}}$ for Gravitational Waves: Consistently Combining Information from Multiple Search Pipelines
• Scalar polarization window in gravitational-wave signals
• Associating fast radio bursts with compact binary mergers via gravitational lensing
• Search for Postmerger Gravitational Waves from Binary Neutron Star Mergers Using a Matched-filtering Statistic
• Where binary neutron stars merge: predictions from IllustrisTNG
• Gravitational Wave Searches for Post-Merger Remnants of GW170817 and GW190425
• Universal relations to measure neutron star properties from targeted r-mode searches
• Half-solution to the two-body problem in General Relativity
• Luminosity distance uncertainties from gravitational wave detections by third generation observatories
• Spin effects in the phasing formula of eccentric compact binary inspirals up to the third post-Newtonian order
• B-modes from Post-inflationary Gravitational Waves Sourced by Axionic Instabilities at Cosmic Reionization
• Dissipative coupling, dispersive coupling and their combination in the cavity-less opto-mechanical systems
• Swift X-ray Follow-Up Observations of Gravitational Wave and High-Energy Neutrino Coincident Signals
• Two-Step Procedure to Detect Cosmological Gravitational Wave Backgrounds with Next-Generation Terrestrial Gravitational-Wave Detectors
• Effects of Galaxy Cluster Structure on Lensed Gravitational Waves
• High-precision source characterization of intermediate mass-ratio black hole coalescences with gravitational waves: The importance of higher-order multipoles
• Probing Ensemble Properties of Vortex-avalanche Pulsar Glitches with a Stochastic Gravitational-Wave Background Search
• Lensing and wave optics in the strong field of a black hole
• A laser interferometer accelerometer for vibration sensitive cryogenic experiments
• The GW-Universe Toolbox III: simulating joint observations of gravitational waves and gamma-ray bursts
• Discriminating same-mass Neutron Stars and Black Holes gravitational wave-forms
• Inferring kilonova population properties with a hierarchical Bayesian framework I : Non-detection methodology and single-event analyses
• Early warning of precessing neutron-star black-hole binary mergers with the near-future gravitational-wave detectors
• Constraining the stochastic gravitational wave background using the future lunar seismometers
• Measuring the Black Hole Mass Spectrum from Redshifts of aLIGO Binary Merger Events
• Graphics processing unit implementation of the F-statistic for continuous gravitational wave searches
• Path integral action for a resonant detector of gravitational waves in the generalized uncertainty principle framework
• Ultralight boson constraints from gravitational wave observations of spinning binary black holes
• Prospects for the observation of continuous gravitational waves from spinning neutron stars lensed by the galactic supermassive black hole
• Confronting general relativity with principal component analysis: Simulations and results from GWTC-3 events
• Slow-rotating charged black hole solution in dynamical Chern-Simons modified gravity
• Astrophysical Source Classification and Distance Estimation for PyCBC Live
• Vibration Analysis of KAGRA Cryostat at Cryogenic Temperature
• How to confirm the existence of population III stars by observations of gravitational waves
• Multidimensional hierarchical tests of general relativity with gravitational waves
• False positives for gravitational lensing: the gravitational-wave perspective
• Quasi-periodic oscillation in short gamma-ray bursts from black hole-neutron star mergers
• Fast Frequency-Domain Effective Fly-By Waveforms
• Effect of Scalar Boson on Fermionic Dark Star
• Search for the optical counterpart of the GW170814 gravitationalwave event with the VLT Survey Telescope
• GWOPS: A VO-technology Driven Tool to Search for the Electromagnetic Counterpart of Gravitational Wave Event
• On the large apparent black hole spin-orbit misalignment angle in GW200115
• Improving the stability of frequency dependent squeezing with bichromatic control of filter cavity length, alignment and incident beam pointing
• Improved early-warning estimates of luminosity distance and orbital inclination of compact binary mergers using higher modes of gravitational radiation
• Observational constraint on axion dark matter in a realistic halo profile with gravitational waves
• Search for stochastic gravitational-wave background from string cosmology with Advanced LIGO and Virgo's O1$\sim$O3 data
• Precessing Binary Black Holes as Better Dark Sirens
• Binary dynamics to second post-Newtonian order in scalar-tensor and Einstein-scalar-Gauss-Bonnet gravity from effective field theory
• Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset
• Data-driven extraction, phenomenology and modeling of eccentric harmonics in binary black hole merger waveforms
• Probing axion-like particles with multimessenger observations of neutron star mergers
• Multimessenger hierarchical triple merger gravitational-wave event pair GW190514-GW190521 inside AGN J124942.3 + 344929
• Methodology for constraining ultralight vector bosons with gravitational wave searches targeting merger remnant black holes
• Gravitational-Wave Parameter Estimation in non-Gaussian noise using Score-Based Likelihood Characterization
• Stable Case BB/BC Mass Transfer to Form GW190425-like Massive Binary Neutron Star Mergers
• Assessing the Impact of Unequal Noises and Foreground Modeling on SGWB Reconstruction with LISA
• Space-based optical lattice clocks as gravitational wave detectors in search for new physics
• Einstein-Klein-Gordon system via Cauchy-characteristic evolution: Computation of memory and ringdown tail
• Post-Newtonian Dynamics of Spinning Black Hole Binaries in Einstein-Scalar-Gauss-Bonnet Gravity
• Projections of the uncertainty on the compact binary population background using popstock
• The curvature dependence of gravitational-wave tests of General Relativity
• Two sides of the same coin: the F-statistic and the 5-vector method
• HERMES: Gamma Ray Burst and Gravitational Wave counterpart hunter
• Bounds on the charge of the graviton using gravitational wave observations
• Impact of gravitational waveform model systematics on the measurement of the Hubble constant
• Eccentricity matters: Impact of eccentricity on inferred binary black hole populations
• Angular correlation and deformed Hellings-Downs curve from spin-2 ultralight dark matter
• Constraints on Brans-Dicke gravity from neutron star-black hole merger events using higher harmonics
• Search for gravitational wave signals from known pulsars in LIGO-Virgo O3 data using the 5n-vector ensemble method
• Phenomenological gravitational waveform model of binary black holes incorporating horizon fluxes
• Piecewise frequency model for searches for long-transient gravitational waves from young neutron stars
• Implications of Pulsar Timing Array Results for High Frequency Gravitational Waves
• Multi-messenger astronomy with a Southern-Hemisphere gravitational-wave observatory
• Effects of a Late Gravitational Transition on Gravitational Waves and Anticipated Constraints
• Constraints on peculiar velocity distribution of binary black holes using gravitational waves with GWTC-3
• The Virtual Research Environment: towards a comprehensive analysis platform
• Distinguishing binary black hole precessional morphologies with gravitational wave observations
• Imaging Scatterometer for Observing In-Situ Changes to Optical Coatings During Air Annealing
• Parameter Distributions of Binary Black Hole Mergers Near Supermassive Black Holes as Seen by Advanced Gravitational Wave Detectors
• LitePIG: A Lite Parameter Inference system for the Gravitational wave in the millihertz band
• Accelerating Tests of General Relativity with Gravitational-Wave Signals using Hybrid Sampling
• Estimation of Newtonian noise from KAGRA cooling system
• Impact of calibration uncertainties on Hubble constant measurements from gravitational-wave sources
• Prospects for reconstructing the gravitational-wave signals from core-collapse supernovae with Advanced LIGO-Virgo and the BayesWave algorithm
• Unveiling the Universe with Emerging Cosmological Probes
• Gravitational Lensing in the Charged NUT-de Sitter Spacetime
• Selection Effects in Periodic X-ray Data from Maximizing Detection Statistics
• Effective chirp mass captures the inspiral frequency evolution of the non-spinning eccentric compact binary
• Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins
• Broadband Dichromatic Variational Measurement
• The missing link in gravitational-wave astronomy: A summary of discoveries waiting in the decihertz range
• A back-linked Fabry-Perot interferometer for space-borne gravitational wave observations
• Topology change and emergent scale symmetry in compact star matter via gravitational wave detection
• Reissner-Nordström perturbation framework with gravitational wave applications
• Compact integrated optical sensors and electromagnetic actuators for vibration isolation systems in the gravitational-wave detector KAGRA
• Cosmological model selection from standard siren detections by third-generation gravitational wave obervatories
• The binary black hole explorer: on-the-fly visualizations of precessing binary black holes
• Enhancing gravitational waveform models through dynamic calibration
• Exploring the distance-redshift relation with gravitational wave standard sirens and tomographic weak lensing
• Light, the universe, and everything -- 12 Herculean tasks for quantum cowboys and black diamond skiers
• Reducing the number of templates for aligned-spin compact binary coalescence gravitational wave searches using metric-agnostic template nudging
• How close can we approach the event horizon of the Kerr black hole from the detection of the gravitational quasinormal modes?
• Beyond the Horizon Distance: LIGO-Virgo can Boost Gravitational Wave Detection Rates by Exploiting the Mass Distribution of Neutron Stars
• Enhancing the sensitivity of interferometers with stable phase-insensitive quantum filters
• Searching for double-peak and doubly broken gravitational-wave spectra from Advanced LIGO-Virgo's first three observing runs
• A new estimation method for mass of an isolated neutron star using gravitational waves
• Model-independent search for anisotropies in stochastic gravitational-wave backgrounds and application to LIGO-Virgo's first three observing Runs
• Hierarchical triple mergers: testing Hawking's area theorem with the inspiral signals
• Semianalytical Approach for Sky Localization of Gravitational Waves
• Assessing the systematic errors of extreme-mass-ratio inspirals waveforms for testing general relativity
• Observability of spin precession in the presence of a black-hole remnant kick
• Navigating Unknowns: Deep Learning Robustness for Gravitational Wave Signal Reconstruction
• Binary dynamics from Einstein-Maxwell theory at second post-Newtonian order using effective field theory
• Reducing controls noise in gravitational wave detectors with interferometric local damping of suspended optics
• Population Synthesis of Black Hole Binaries with Compact Star Companions
• Minimally-modeled search of higher multipole gravitational-wave radiation in compact binary coalescence
• A High-Finesse Suspended Interferometric Sensor for Macroscopic Quantum Mechanics with Femtometre Sensitivity
• The origin channels of hierarchical binary black hole mergers in the LIGO-Virgo-KAGRA O1, O2, and O3 runs
• Linear dynamics and classical tests of the gravitational quantum field theory
• On exotic objects made of dark energy and dark matter: Mass-to-radius profiles and tidal Love numbers
• Search for continuous gravitational waves from HESS~J1427-608 with a hidden Markov model
• Minimally modified gravity with auxiliary constraints formalism
• High Speed Source Localization in Searches for Gravitational Waves from Compact Object Collisions
• The effect of noise artefacts on gravitational-wave searches for neutron star post-merger remnants
• Characterization of gravitational-wave detector noise with fractals
• Memory of a Random Walk: Astrometric deflections from gravitational wave memory accumulation over cosmological scales
• Can we use next-generation gravitational wave detectors for terrestrial precision measurements of Shapiro delay?
• Determination of compressive stress in thin films using micro-machined buckled membranes
• Astrophysics with the Laser Interferometer Space Antenna
• What do gravitational wave detectors say about polymer quantum effects?
• Reconstruction of binary black hole harmonics in LIGO using deep learning
• Validating Sequential Monte Carlo for Gravitational-Wave Inference
• Development of wide-field low-energy X-ray imaging detectors for HiZ-GUNDAM
• Inferring small neutron star spins with neutron star-black hole mergers
• Prospects for Time-Domain and Multi-Messenger Science with eXTP
• Numerical Relativity Multimodal Waveforms using Absorbing Boundary Conditions
• Binary Neutron Star Merger Search Pipeline Powered by Deep Learning
• cDVGAN: One Flexible Model for Multi-class Gravitational Wave Signal and Glitch Generation
• A nested sampling code for targeted searches for continuous gravitational waves from pulsars
• Design of Microresonators to Minimize Thermal Noise Below the Standard Quantum Limit
• Automated Evaluation of Environmental Coupling for Advanced LIGO Gravitational Wave Detections
• Constraints on ultra-low-frequency gravitational waves with statistics of pulsar spin-down rates
• GPU-accelerated Image Reduction Pipeline
• Eccentricity evolution consistency test to distinguish eccentric gravitational-wave signals from eccentricity mimickers
• Search for continuous gravitational waves directed at sub-threshold radiometer candidates in O3 LIGO data
• No Glitch in the Matrix: Robust Reconstruction of Gravitational Wave Signals Under Noise Artifacts
• Detecting and reconstructing gravitational waves from the next Galactic core-collapse supernova in the Advanced Detector Era
• Gravitational waves from cosmic strings for pedestrians
• Gravitational waves and galaxies cross-correlations: a forecast on GW biases for future detectors
• Biased parameter inference of eccentric, spin-precessing binary black holes
• Angular instability in high optical power suspended cavities
• Characterizing the effect of eccentricity on the dynamics of binary black hole mergers in numerical relativity
• Targeted Search for Gravitational Waves from Highly Spinning Light Compact Binaries
• The Timing System of LIGO Discoveries
• Bayesian Analysis of the Neutron Star Equation of State and Model Comparison: Insights from PSR J0437+4715, PSR J0614+3329, and Other Multi-Physics Data
• Efficient method for measuring the parameters encoded in a gravitational-wave signal
• Interaction between linear polarized plane gravitational waves and a plane electromagnetic wave in the electromagnetic-gravity analogue
• Scalar-Induced Gravitational Waves in a $\Lambda$CDM Cosmology
• Dual balanced readout for scattered light noise mitigation in Michelson interferometers
• Point Absorber Limits to Future Gravitational-Wave Detectors
• A Common Origin for Low Mass Ratio Events Observed by LIGO and Virgo in the First Half of the Third Observing Run
• First-step experiment in developing optical-spring quantum locking for DECIGO: sensitivity optimization for simulated quantum noise by completing the square
• Waging a Campaign: Results from an Injection-Recovery Study involving 35 numerical Relativity Simulations and three Waveform Models
• A Deep Learning Powered Numerical Relativity Surrogate for Binary Black Hole Waveforms
• Gravitational-Wave Signatures of Nonstandard Neutrino Properties in Collapsing Stellar Cores
• Cosmic Cartography II: completing galaxy catalogs for gravitational-wave cosmology
• Inferring black-hole orbital dynamics from numerical-relativity gravitational waveforms
• Stochastic Gravitational Wave Background from PBH-ABH Mergers
• Testing the validity of the phenomenological gravitational waveform models for nonspinning binary black hole searches at low masses
• Optimizing Neural Network Surrogate Models: Application to Black Hole Merger Remnants
• Constraining Black Hole Populations in Globular Clusters using Microlensing: Application to Omega Centauri
• Modeling Gravitational Wave Modes from the Inspiral of Binaries with Arbitrary Eccentricity
• Tunable coherence laser interferometry: demonstrating 40dB of straylight suppression and compatibility with resonant optical cavities
• Seeking Spinning Subpopulations of Black Hole Binaries via Iterative Density Estimation
• Probing Self-Interacting Dark Matter via Gravitational-Wave Background from Eccentric Supermassive Black Hole Mergers
• Diffraction around caustics in gravitational wave lensing
• Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression
• Multi-messenger observations in the Einstein Telescope era: binary neutron star and black hole - neutron star mergers
• Probing Particle Physics with Gravitational Waves
• A directed continuous-wave search from Scorpius X-1 with the five-vector resampling technique
• Driving unmodelled gravitational-wave transient searches using astrophysical information
• Taming systematics in distance and inclination measurements with gravitational waves: role of the detector network and higher-order modes
• Accelerating the standard siren method: Improved constraints on modified gravitational-wave propagation with future data
• Probing the large-scale structure of the universe through gravitational-wave observations
• Fast Simulation of Gaussian-Mode Scattering for Precision Interferometry
• Recent LIGO-Virgo discoveries
• A high angular resolution interferometric backscatter meter
• Combination of dissipative and dispersive coupling in the cavity optomechanical systems
• Investigating the detection rates and inference of gravitational-wave and radio emission from black hole neutron star mergers
• Radio Constraints on $r$-process Nucleosynthesis by Collapsars
• Search for Coincident Gravitational Wave and Long Gamma-Ray Bursts from 4-OGC and the Fermi-GBM/Swift-BAT Catalog
• Observational constraint on axion dark matter with gravitational waves
• Dipole Anisotropy in Gravitational Wave Source Distribution
• X- and Gamma-ray astrophysics in the era of Multi-messenger astronomy
• Exposing Gravitational Waves below the Quantum Shot Noise
• Comparison and application of different post-Newtonian models for inspiralling stellar-mass binary black holes with space-based GW detectors
• Response of the underground environment of the KAGRA observatory against the air-pressure disturbance from the Tonga volcano eruption on January 15th, 2022
• Success of the small mass ratio approximation during the final orbits of binary black hole simulations
• Optical losses as a function of beam position on the mirrors in a 285-m suspended Fabry-Perot cavity
• Probing intermediate scale Froggatt-Nielsen models at future gravitational wave observatories
• Revisiting Thermal Charge Carrier Refractive Noise in Semiconductor Optics for Gravitational-Wave Interferometers
• An instrumented baffle for the Advanced Virgo Input Mode Cleaner End Mirror
• Probing cosmic chemical enrichment with next-generation gravitational-wave observatories
• A complete measurement of a black-hole recoil through higher-order gravitational-wave modes
• The capability of the Australian Square Kilometre Array Pathfinder to detect prompt radio bursts from neutron star mergers
• Searching for Gravitational-Wave Counterparts using the Transiting Exoplanet Survey Satellite
• Optimal Gravitational-wave Follow-up Tiling Strategies Using a Genetic Algorithm
• Gas cooling of test masses for future gravitational-wave observatories
• Quasinormal Modes by Improved Matrix Method and Weighted Residual Method
• Novel Deep Learning Approach to Detecting Binary Black Hole Mergers
• Impact of Bayesian Priors on the Inferred Masses of Quasi-Circular Intermediate-Mass Black Hole Binaries
• Early Advanced LIGO binary neutron-star sky localization and parameter estimation
• Background information: a study on the sensitivity of astrophysical gravitational-wave background searches
• Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds. II. Subthreshold binary neutron stars
• TOROS Optical follow-up of the Advanced LIGO-VIRGO O2 second observational campaign
• New semicoherent targeted search for continuous gravitational waves from pulsars in binary systems
• A Three-Dimensional Laser Interferometer Gravitational-Wave Detector
• Detection of GW200105 with a targeted eccentric search
• lenscat: a Public and Community-Contributed Catalog of Known Strong Gravitational Lenses
• High Frame-Rate Phase Camera for High-Resolution Wavefront Sensing in Gravitational-Wave Detectors
• Prospects of constraining on the polarizations of gravitational waves from binary black holes using space- and ground-based detectors
• Passive-performance, analysis, and upgrades of a 1-ton seismic attenuation system
• Demonstration of a dual-pass differential Fabry-Perot interferometer for future interferometric space gravitational wave antennas
• Gravitational Wave Detection via Weak Measurements Amplification
• Integrating high-precision and fringe-scale displacement sensing using heterodyne cavity-tracking
• Next-generation global gravitational-wave detector network: Impact of detector orientation on compact binary coalescence and stochastic gravitational-wave background searches
• Origin of Black Hole Spin in Lower-Mass-Gap Black Hole-Neutron Star Binaries
• Accelerated parameter estimation of supermassive black hole binaries in LISA using a meshfree approximation
• Efficiency of nonspinning templates in gravitational wave searches for aligned-spin binary black holes
• A search using GEO600 for gravitational waves coincident with fast radio bursts from SGR 1935+2154
• Calibration of Advanced Virgo and reconstruction of detector strain h(t) during the Observing Run O3
• GW230814: investigation of a loud gravitational-wave signal observed with a single detector
• Gravitational Wave Searches for Aligned-Spin Binary Neutron Stars Using Nonspinning Templates
• Search for gravitational waves from eccentric binary black holes with an effective-one-body template
• Gravitational Wave From Axion-like Particle Inflation
• A complete waveform comparison of post-Newtonian and numerical relativity in eccentric orbits
• Scalar Gravitational Wave Signals from Core Collapse in Massive Scalar-Tensor Gravity with Triple-Scalar Interactions
• Trajectories without quantum uncertainties in composite systems with disparate energy spectra
• Analytic weak-signal approximation of the Bayes factor for continuous gravitational waves
• Neutron Stars, Ungravity, and the I-Love-Q relation
• Nonlinear noise regression in gravitational-wave detectors with convolutional neural networks
• Polarization Properties of the Electromagnetic Response to High-frequency Gravitational Wave
• Effects of Short-Distance Modifications to General Relativity in Spinning Binary Systems
• Stochastic gravitational wave background from supernovae in massive scalar-tensor gravity
• WINTER on S250206dm: A near-infrared search for an electromagnetic counterpart to a gravitational-wave event
• The directional isotropy of LIGO-Virgo binaries
• Spectrogram correlated stacking: A novel time-frequency domain analysis of the Stochastic Gravitational Wave Background
• Machine Learning for Quantum-Enhanced Gravitational-Wave Observatories
• Estimate of the Detectability of the Circular Polarisation Signature of Supernova Gravitational Waves Using the Stokes Parameters
• Towards optomechanical parametric instabilities prediction in ground-based gravitational wave detectors
• Data-driven approach for modeling the temporal and spectral evolution of kilonova systematic uncertainties
• Gravitational light deflection in Earth-based laser cavity experiments
• Measuring Gravitational Wave Speed and Lorentz Violation with the First Three Gravitational-Wave Catalogs
• Inferring astrophysics and cosmology with individual compact binary coalescences and their gravitational-wave stochastic background
• Inferring spin tilts of binary black holes at formation with plus-era gravitational wave detectors
• Comparison of neural network architectures for feature extraction from binary black hole merger waveforms
• Population synthesis and parameter estimation of neutron stars with continuous gravitational waves and third-generation detectors
• Phase decomposition of the template metric for continuous gravitational-wave searches
• Deep learning-based astronomical multimodal data fusion: A comprehensive review
• Probing eccentric higher-order modes through an effective chirp mass model
• Searching for Anisotropy in the Gravitational Wave Background Using the Parkes Pulsar Timing Array
• Estimate of the radius responsible for quasinormal modes in the extreme Kerr limit and asymptotic behavior of the Sasaki-Nakamura transformation
• The impact of local noise recorded at the ET candidate sites on the signal to noise ratio of CBC gravitational wave signals for the ET triangle configuration
• Colloquium: Multimessenger astronomy with continuous gravitational waves and future detectors
• Parametrized multipolar gravitational waveforms for testing general relativity: Amplitude corrections up to 2PN order
• Optimized localization for gravitational-waves from merging binaries
• Probing black hole `charge' from the binary black hole inspiral
• Gravitational wave imprints on spontaneous emission
• Classification uncertainty for transient gravitational-wave noise artefacts with optimised conformal prediction
• Detectability of Gravitational-Wave Memory with LISA: A Bayesian Approach
• Looking To The Horizon: Probing Evolution in the Black Hole Spectrum With Gravitational Wave Catalogs
• Uncovering faint lensed gravitational-wave signals and reprioritizing their follow-up analysis using galaxy lensing forecasts with detected counterparts
• Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements
• Strong lensing of gravitational waves with modified propagation
• DeepExtractor: Time-domain reconstruction of signals and glitches in gravitational wave data with deep learning
• Energy flux and waveform of gravitational wave generated by coalescing slow-spinning binary system in effective one-body theory
• The linear stability of the post-Newtonian triangular equilibrium in the three-body problem
• Systematic Bias Due to Nonspinning Template Waveforms in the Gravitational Wave Parameter Estimation for Aligned-Spin Binary Black Holes
• Random projections in gravitational wave searches of compact binaries
• Constraining parameters of low mass merging compact binary systems with Einstein Telescope alone
• Profiling stellar environments of gravitational wave sources
• Folding Gravitational-Wave Interferometers
• Are long gamma-ray bursts progenitors to merging binary black holes?
• Simplified optical configuration for a sloshing-speedmeter-enhanced gravitational wave detector
• Arm locking in conjunction with time-delay interferometry
• Expediting DECam Multimessenger Counterpart Searches with Convolutional Neural Networks
• Identifying multichannel coherent couplings and causal relationships in gravitational wave detectors
• Design and experimental demonstration of a laser modulation system for future gravitational-wave detectors
• Scattering Loss in Precision Metrology due to Mirror Roughness
• Strategies to reduce the thermoelastic loss of multimaterial coated finite substrates
• Constraining self-interactions of a massive scalar field using scalar gravitational waves from stellar core collapse
• Observing the optical modes of parametric instability
• Assessing the similarity of continuous gravitational-wave signals to narrow instrumental artifacts
• Broadband Coherent Multidimensional Variational Measurement
• Cosmology in the dark: How compact binaries formation impact the gravitational-waves cosmological measurements
• Scalar fields around black hole binaries in LIGO-Virgo-KAGRA
• Review of Conformally Flat Approximation for Binary Neutron Star Initial Conditions
• A novel multi-layer modular approach for real-time fuzzy-identification of gravitational-wave signals
• Gravitational waves from superradiant instabilities of rotating black holes
• Improving LIGO calibration accuracy by using time-dependent filters to compensate for temporal variations
• Post-newtonian analysis of precessing convention for spinning compact binaries
• Can a "pure vector" gravitational wave mimic a "pure tensor" one?
• Numerical-relativity surrogate modeling with nearly extremal black-hole spins
• A follow-up on intermediate-mass black hole candidates in the second LIGO-Virgo observing run with the Bayes Coherence Ratio
• UniMAP: Model-free detection of unclassified noise transients in LIGO-Virgo data using the Temporal Outlier Factor
• Probing Fundamental Physics with Gravitational Waves
• Accounting for the Known Unknowns: A Parametric Framework to Incorporate Systematic Waveform Errors in Gravitational-Wave Parameter Estimation
• Measuring the speed of gravity and the cosmic expansion with time delays between gravity and light from binary neutron stars
• Regularization of a scalar charged particle for generic orbits in Kerr spacetime
• Thermal noise of beam splitters in laser gravitational wave detectors
• Quantum Bayesian Inference with Renormalization for Gravitational Waves
• Robust, Rapid, and Simple Gravitational-wave Parameter Estimation
• Cold Atoms in Space: Community Workshop Summary and Proposed Road-Map
• A characterization method for low-frequency environmental noise in LIGO
• Mapping Parameter Correlations in Spinning Binary Black Hole Mergers
• Robust and fast parameter estimation for gravitational waves from binary neutron star merger remnants
• Waveform Reconstruction of Core-Collapse Supernova Gravitational Waves with Improved Multisynchrosqueezing Transform
• Repeated Bursts: Gravitational Waves from Highly Eccentric Binaries
• Gravitational-wave signatures of mirror (a)symmetry in binary black hole mergers: measurability and correlation to gravitational-wave recoil
• An Interactive Gravitational-Wave Detector Model for Museums and Fairs
• Learning Transient Universe in Near-Ultraviolet By Wide-angle Cameras
• Searches for continuous gravitational waves from young supernova remnants in the early third observing run of Advanced LIGO and Virgo
• The Gravitational-wave Optical Transient Observer (GOTO): prototype performance and prospects for transient science
• Gravitational-wave model for neutron star merger remnants with supervised learning
• Photothermal effect in macroscopic optomechanical systems with an intracavity nonlinear optical crystal
• Are all models wrong? Falsifying binary formation models in gravitational-wave astronomy
• Gravitational waves from eccentric binary neutron star mergers: Systematic biases and inadequacy of quasicircular templates
• Reassessing the Spin of Second-born Black Holes in Coalescing Binary Black Holes and Its Connection to the chi_eff-q Correlation
• Improved binary black hole searches through better discrimination against noise transients
• Effects of calibration uncertainties on the detection and parameter estimation of isotropic gravitational-wave backgrounds
• Sky localization of space-based detectors with time-delay interferometry
• GW231123: Overlapping Gravitational Wave Signals?
• Measuring $H_0$ with pulsar timing arrays
• The Nature of Gravitational Wave Events with Host Environment Escape Velocities
• Development of advanced photon calibrator for Kamioka gravitational wave detector (KAGRA)
• Black-Hole Cartography
• Maximum mass and stability of differentially rotating neutrons stars
• Prospects for estimating parameters from gravitational waves of superspinar binaries
• Probing Binary Lens Caustics with Gravitational Waves: A Uniform Approximation Approach
• Thermal evolution of dark matter and gravitational-wave production in the early universe from a symplectic glueball model
• Gravitational lensing aided luminosity distance estimation for compact binary coalescences
• Optimal Design of Coatings for Mirrors of Gravitational Wave Detectors: Analytic Turbo Solution via Herpin Equivalent Layers
• Wavelet graphs for the direct detection of gravitational waves
• Investigation of crackling noise in the vibration isolation systems of the KAGRA gravitational wave detector
• Inferring the spins of merging black holes in the presence of data-quality issues
• Testing hilltop supernatural inflation with gravitational waves
• Study of selected mild steels for application in vacuum systems of future gravitational wave detectors
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Deep Multimessenger Search for Compact Binary Mergers in LIGO, Virgo, and Fermi/GBM Data from 2016-2017
• Extending the short gamma-ray burst population from sub-threshold triggers in Fermi/GBM and GECAM data and its implications
• Cosmology with Binary Neutron Stars: Does Mass-Redshift Correlation Matter?
• Global Stellar Budget for LIGO Black Holes
• The Response of Laser Interferometric Gravitational Wave Detectors Beyond the Eikonal Equation
• What to expect: kilonova light curve predictions via equation of state marginalization
• High Dynamic Range Spatial Mode Decomposition
• Rates and beaming angles of GRBs associated with compact binary coalescences
• Numerical Relativity Estimates of the Remnant Recoil Velocity in Binary Neutron Star Mergers
• Unified laboratory-frame analysis of atomic gravitational-wave sensors
• Self-calibration of Networks of Gravitational Wave Detectors
• Status of the Advanced Virgo gravitational-wave detector
• Evidence for Three Subpopulations of Merging Binary Black Holes at Different Primary Masses
• Obtaining Statistical Significance of Gravitational Wave Signals in Hierarchical Search
• Electroweak Phase Transition, Gravitational Waves and Collider Probes in Multi-Scalar Dark Matter Scenarios
• Chiral gravitational waves from thermalized neutrinos in the early Universe
• Derivative of the light frequency shift as a measure of spacetime curvature for gravitational wave detection
• Testing modified gravity with the eccentric neutron star--black hole merger GW200105
• On the Astrophysical Origin of Binary Black Hole Subpopulations: A Tale of Three Channels?
• Generative adversarial network for stellar core-collapse gravitational waves
• A prototype differential atom interferometer for fundamental physics
• Joint inference for gravitational wave signals and glitches using a data-informed glitch model
• Multi-messenger searches via IceCube's high-energy neutrinos and gravitational-wave detections of LIGO/Virgo
• Conceptual design and science cases of a juggled interferometer for gravitational wave detection
• Detecting and Diagnosing Terrestrial Gravitational-Wave Mimics Through Feature Learning
• Deep insights into the local structure of amorphous Ta2O5 thin films by X-ray pair distribution function analysis
• Atmospheric Newtonian noise modeling for third-generation gravitational wave detectors
• Exploring the Potential for Detecting Rotational Instabilities in Binary Neutron Star Merger Remnants with Gravitational Wave Detectors
• Gravitational wave signals from long lasting binary-single black hole encounters
• Application of a new transient-noise analysis tool for an unmodeled gravitational-wave search pipeline
• Sensing and vetoing loud transient noises for the gravitational-wave detection
• The Use of Binary Black Holes Merging in AGN Disks for Hubble Constant Measurements
• Interpreting gravitational-wave burst detections: constraining source properties without astrophysical models
• Optimizing the low-latency localization of gravitational waves
• All-sky search for long-duration gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run
• Probing Spin-Orbit Resonances with the Binary Black Hole Population
• Quantum sensors with matter waves for GW observation
• Probing Cosmology with Baryon Acoustic Oscillations using Gravitational Waves
• Binary Neutron Star (BNS) merger: What we learned from relativistic ejecta of GW/GRB~170817A
• Chirp mass based glitch identification in long duration gravitational wave transients
• Limits on the Stochastic Gravitational Wave Background and Prospects for Single Source Detection with GRACE Follow-On
• Multi-Messenger Astrophysics with THESEUS in the 2030s
• Dynamical friction from scalar dark matter in the relativistic regime
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Nonlinear mode-tide coupling in coalescing binary neutron stars with relativistic corrections
• Implementation of the rROF denoising method in the cWB pipeline for gravitational-wave data analysis
• Perspectives for multi-messenger astronomy with the next generation of gravitational-wave detectors and high-energy satellites
• Characterization of ion-beam-sputtered AlF${}_3$ thin films for gravitational-wave interferometers
• Displacement-noise-free interferometeric gravitational-wave detector using unidirectional neutrons with four speeds
• Rapid Hierarchical Inference of Neutron Star Equation of State from multiple Gravitational Wave Observations of Binary Neutron Star Coalescences
• A Pseudo Plane-wave Gravitational Calibrator for Gravitational Wave Observatories
• Gravitational wave signatures from the phase-transition-induced collapse of a magnetized neutron star
• Beam displacement tolerances on a segmented mirror for higher-order Hermite-Gauss modes
• Enhanced optomechanical interaction in the unbalanced interferometer
• Sensing and control scheme for the inteferometer configuration with an L-shaped resonator
• Probing the equation of state of neutron stars with captured primordial black holes
• Constraining Electromagnetic Signals from Black Holes with Hair
• Single-event likelihood of star cluster properties with LIGO-Virgo-Kagra binary black hole observations
• Machine-directed gravitational-wave counterpart discovery
• Searching for topological dark matter in LIGO data
• Self-consistent treatment of thermal effects in neutron-star post-mergers: observational implications for third-generation gravitational-wave detectors
• Unmasking noise transients masquerading as intermediate-mass black hole binaries
• Do black holes remember what they are made of?
• Digital Discovery of interferometric Gravitational Wave Detectors
• Efficient prescription to search for linear gravitational wave memory from hyperbolic black hole encounters and its application to the NANOGrav 12.5-year dataset
• Mass function of stellar black holes as revealed by the LIGO-Virgo-KAGRA observations
• Effect of spin in binary neutron star mergers
• Small Spins of Primordial Black Holes from Random Geometries: Bekenstein-Hawking Entropy and Gravitational Wave Observations
• Tests of general relativity at the fourth post-Newtonian order
• Can the Near-Horizon Black Hole Memory be detected through Binary Inspirals?
• Rapid Parameter Estimation for Merging Massive Black Hole Binaries Using Continuous Normalizing Flows
• Joint Inference of Population, Cosmology, and Neutron Star Equation of State from Gravitational Waves of Dark Binary Neutron Stars
• Enhancing gravitational-wave host localization with SKYFAST: rapid volume and inclination angle reconstruction
• A weakly-modeled search for compact binary coalescences in Einstein Telescope
• Search for a Gravitational-Wave Background from Sound Speed Resonance from Advanced LIGO and Advanced Virgo's First Three Observing Runs
• Hierarchical searches for subsolar-mass binaries and the third-generation gravitational wave detector era
• Effects of orbital eccentricity on continuous gravitational waveforms from triaxially deformed precessing neutron stars in tight binaries
• On the use of galaxy catalogs in gravitational-wave parameter estimation
• Search for exotic gravitational wave signals beyond general relativity using deep learning
• Compact object populations over cosmic time I. BOSSA: a Binary Object environment-Sensitive Sampling Algorithm
• Can Neutron Star Tidal Effects Obscure Deviations from General Relativity?
• One-stop strategy to search for long-duration gravitational-wave signals
• Inferring jet physics from neutron star - black hole mergers with gravitational waves
• Detecting Unmodeled, Source-dependent Signals in Gravitational Waves with SCoRe
• Using t-SNE for characterizing glitches in LIGO detectors
• Theoretical Radio Signals from Radio-Band Gravitational Waves Converted from the Neutron Star Magnetic Field
• An analytical joint prior for effective spins for inference on the spin distribution of binary black holes
• Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers
• Surrogate modeling of gravitational waves microlensed by spherically symmetric potentials
• Constraining black-hole horizon effects by LIGO-Virgo detections of inspiralling binary black holes
• Sky localization of gravitational waves from eccentric binaries
• Effect of kick velocity on gravitational wave detection of binary black holes with space- and ground-based detectors
• Quantum Interference in Atomic Systems
• Limits on the existence of totally reflective exotic compact objects with current and future gravitational-wave detectors
• Thermal X-ray signatures in late-stage unequal-mass massive black hole binary mergers
• Accelerating the time-domain LISA response model with central finite differences and hybridization techniques
• Imprints of Non-Symmetric Dark Matter Halos on Magnetars: A Two-Fluid Perspective
• Complete Catalog of Laser Locking Configurations for LISA
• Glitches far from transient gravitational-wave events do not bias inference
• A pipeline to search for signatures of line-of-sight acceleration in gravitational wave signals produced by compact binary coalescences
• Detection probability of light compact binary mergers in future observing runs of the current ground-based gravitational wave detector network
• Overlapping signals in next-generation gravitational wave observatories: A recipe for selecting the best parameter estimation technique
• Reanalysis of LIGO black-hole coalescences with alternative prior assumptions
• Comparing astrophysical models to gravitational-wave data in the observable space
• RADAR-Radio Afterglow Detection and AI-driven Response: A Federated Framework for Gravitational Wave Event Follow-Up
• Transformer Networks for Continuous Gravitational-wave Searches
• Echoes from the dark: Galaxy catalog incompleteness in standard siren cosmology
• Expect the unexpected: augmented mixture models for black-hole-population studies
• Effects of dynamical capture on two equal-mass nonspinning black holes
• Ten years of extreme gravity tests of general theory of relativity with gravitational-wave observations
• Testing general relativity with gravitational waves -- improving and extending Modified Dispersion Relation tests
• Testing general relativity with amplitudes of subdominant gravitational-wave modes
• Computing spectral shifts for Johannsen-Psaltis black holes
• Discovering gravitational waveform distortions from lensing: A deep dive into GW231123
• Beyond FINDCHIRP: Breaking the memory wall and optimal FFTs for Gravitational-Wave Matched-Filter Searches with Ratio-Filter Dechirping
• Fast response electromagnetic follow-ups from low latency GW triggers
• Systematic errors in low latency gravitational wave parameter estimation impact electromagnetic follow-up observations
• How much spin wandering can continuous gravitational wave search algorithms handle?
• Evolutionary tracks of binary neutron star progenitors across cosmic times
• Impact of noise transients on gravitational-wave burst detection efficiency of the BayesWave pipeline with multi-detector networks
• Study of statistical properties of hybrid statistic in coherent multi-detector compact binary coalescences Search
• Boosting the Efficiency of Parametric Detection with Hierarchical Neural Networks
• Measurability of neutron star tidal deformability from merging neutron star-black hole binaries
• Orbital effects due to gravitational induction
• Experimental investigation of the limitations of polarisation optics for future gravitational wave detectors based on the polarisation Sagnac speedmeter
• Multi-Messenger Astrophysics Opportunities with Stellar-Mass Binary Black Hole Mergers
• Multimessenger Probes of High-energy Sources
• Diffraction losses of a Fabry-Perot cavity with nonidentical non-spherical mirrors
• Characterizing Compact-object Binaries in the Lower Mass Gap with Gravitational Waves
• Constraining the abundance of spinning deformed Galactic compact objects with continuous gravitational waves
• Overlap reduction function for gravitational wave detectors in an expanding Universe
• Measurement of the central Galactic black hole by extremely large mass-ratio inspirals
• High-efficiency Electro-Optic Lens for radio frequency beam wavefront modulation for mode mismatch sensing
• Uncertainty and bias of cosmology and astrophysical population model from statistical dark sirens
• A comprehensive look into the accuracy of SpEC binary black hole waveforms
• Performance comparison of multi-detector detection statistics in targeted compact binary coalescence GW search
• GWAI: Artificial Intelligence Platform for Enhanced Gravitational Wave Data Analysis
• Hierarchical Merger of Primordial Black Holes in Dwarf Galaxies
• Quasinormal modes from numerical relativity with Bayesian inference
• Revisiting Singlet Fermion Dark Matter with a Scalar Portal: Connecting Higgs Phenomenology and Strong Electroweak Phase Transition
• Peak energy--Isotropic Luminosity Correlation and Jet Opening Angle Evolution in Swift-BAT Short GRBs with Soft Tail Emission
• GW250114 reveals black hole horizon signatures
• Constraining the Luminosity Function and Delay-Time Distribution of Short Gamma-Ray Bursts for Multimessenger Gravitational-Wave Detection Rate Estimation
• Spontaneous baryogenesis and generation of gravitational waves in a new model of quintessential $\alpha$-attractor
• Gravitational-wave matched filtering on a quantum computer
• First measurement of the Hubble constant from a combined weak lensing and gravitational-wave standard siren analysis
• Gravitational wave quasinormal mode from Population III massive black hole binaries in various models of population synthesis
• Relative calibration of the LIGO and Virgo detectors using astrophysical events from their third observing run
• Implications of the binary coalescence events found in O1 and O2 for the stochastic background of gravitational events
• Numerical simulations of oscillating and differentially rotating neutron stars
• Constraints on gravitational waves from the 2024 Vela pulsar glitch
• A Gaussian process framework for testing general relativity with gravitational waves
• Signatures of Hierarchical Mergers in Black Hole Spin and Mass distribution
• Impact of ultralight bosonic dark matter on the dynamical bar-mode instability of rotating neutron stars
• Deep follow-up for gravitational-wave inference: a case study with GW151226
• Reducing systematic uncertainties in gravitational-wave population analyses by increasing the detection threshold
• Measurement prospects for the pair-instability mass cutoff with gravitational waves
• Architectural Optimization and Feature Learning for High-Dimensional Time Series Datasets
• Accelerating gravitational-wave parameterized tests of General Relativity using a multiband decomposition of likelihood
• Methods for Estimating Neutron Star Parameters using Multiple Mechanisms for Gravitational Wave Emission Associated with Pulsar Glitches
• Finite state machine controls for a source of optical squeezed vacuum
• Can the phase of radiation pressure fluctuations be flipped in a single path for laser interferometric gravitational wave detectors?
• Atom interferometers and a small-scale test of general relativity
• Measurement of the Hubble constant using the Dark Energy Survey Year 6 Gold galaxy catalogue and the fourth Gravitational-Wave Transient Catalogue
• High speed, high power 2D beam steering for mitigation of optomechanical parametric instability in gravitational wave detectors
• Astrophysical constraints on neutron star $f$-modes with a nonparametric equation of state representation
• Statistically-informed deep learning for gravitational wave parameter estimation
• Scalable matched-filtering pipeline for gravitational-wave searches of compact binary mergers
• Evidence of large recoil velocity from a black hole merger signal
• A gating-and-inpainting perspective on GW150914 ringdown overtone: understanding the data analysis systematics
• Comprehensive analysis of dissipative effects in the induced gravitational waves
• Learning to detect continuous gravitational waves: an open data-analysis competition
• Design and optimisation of linear variable differential transformers and voice coil actuators using finite element analysis: a methodical approach to enhance sensor response and actuation force
• Investigation of Mechanical Properties of Cryogenically Treated Music Wire
• Prospects for High-Frequency Gravitational-Wave Detection with GEO600
• Modeling the Beam of Gravitational Radiation from a Cosmic String Loop
• ASAS-SN search for optical counterparts of gravitational-wave events from the third observing run of Advanced LIGO/Virgo
• Multivariate Time Series Clustering for Environmental State Characterization of Ground-Based Gravitational-Wave Detectors
• Using overlap of sky localization probability maps for filtering potentially lensed pairs of gravitational-wave signals
• Gravitational-wave echoes from spinning exotic compact objects: numerical waveforms from the Teukolsky equation
• Complementary signatures of $\alpha -$attractor inflation in CMB and cosmic string Gravitational Waves
• Resonant behavior and stability of a linear three-mirror cavity
• Probing baryogenesis with gravitational waves
• Application of Non-Linear Noise Regression in the Virgo Detector
• Multimessenger Analysis Strategy for Core-Collapse Supernova Search: Gravitational Waves and Low-energy Neutrinos
• Modeling of optical scattering from topographic surface measurements of high-quality mirrors
• $\beta$-Annealed Variational Autoencoder for glitches
• Binary black holes in the heat of merger
• Bounding dark charges on binary black holes using gravitational waves
• Can Big Black Holes Merge with the Smallest Black Holes?
• The impact of precession and higher-order multipoles for gravitational wave cosmological inference
• General Fourier expansion of post-Newtonian binary dynamics based on a quasi-Keplerian framework
• Thermal Deformation Reduction in High-Power Interferometry with Higher-Order Laser Modes
• A 4.5-s Quasiperiodic Spectral Oscillation in GRB 230307A: Evidence for Free Precession of a Post-Merger Magnetar?
• Convection signatures in early-time gravitational waves from core-collapse supernovae
• Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA
• Search for high-frequency gravitational waves via re-analysis of cavity axion data
• The Virgo Newtonian calibration system for the O4 observing run
• Simulation Study on Constraining GW Propagation Speed by GW and GRB Joint Observation on Binary Neutron Star Mergers
• Extremely High-Order Convergence in Simulations of Relativistic Stars
• Resonant amplification of multimessenger emission in rotating stellar core collapse
• Astrophysical and Cosmological Relevance of the High-Frequency Features in the Stochastic Gravitational-Wave Background
• Importance of relativistic pericenter precession in identifying the presence of a third body near eccentric binaries
• Strain sensitivity enhancement in a Grover-Michelson interferometer
• Flexible Gravitational-Wave Parameter Estimation with Transformers
• Towards asteroseismology of neutron stars with physics-informed neural networks
• Proto-neutron star oscillations including accretion flows
• Gravitational Waves and Neutrinos
• Mechanical Characterisation of Silicon for the ETpathfinder Test Masses
• Searching for continuous gravitational waves from highly deformed compact objects with DECIGO
• Group equivariant neural posterior estimation
• Constraining scalar-tensor theories from higher harmonics with GW230529
• Learning and Interpreting Gravitational-Wave Features from CNNs with a Random Forest Approach
• Probing cosmic strings via gravitational-wave lensing
• Doppler correlation-driven vetoes for the Frequency Hough analysis in continuous gravitational-wave searches
• Kilonova and progenitor properties of merger-driven gamma-ray bursts
• Axion Dark Matter Archaeology with Primordial Gravitational Waves
• Banks of templates for directed and all-sky narrow-band searches of continuous gravitational waves from spinning neutron stars with several spindowns
• Exploring future synergies for large-scale structure between gravitational waves and radio sources
• Imprints of an early matter-dominated era arising from dark matter dilution mechanism on cosmic string dynamics and gravitational wave signatures
• Development of a polarimetry method toward in-situ substrate birefringence characterization of ground-based gravitational wave detectors
• Optimizing signal recycling for detecting a stochastic gravitational-wave background
• The Classical Harmonic Vibrations of the Atomic Centers of Mass with Micro Amplitudes and Low Frequencies Monitored by the Entanglement between the Two Two-level Atoms in a Single mode Cavity
• Improved Binary Black Hole Search Discriminator from the Singular Value Decomposition of Non-Gaussian Noise Transients
• Target-based Optimization of Advanced Gravitational-Wave Detector Network Operations
• A ${\chi }^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences
• Fighting Newtonian Noise with Gradient-Based Optimization at the Einstein Telescope
• 3D Localization of FRB 20190425A for Its Potential Host Galaxy and Implications
• Scattered light reduction in Sagnac Speed Meters with Tunable Coherence
• Bispectrum of induced gravitational waves in the poltergeist mechanism
• Evaluation of microseismic motion at the KAGRA site based on ocean wave data
• The influence of the mean anomaly on the dynamical quantities of binary black hole mergers in eccentric orbits
• Polarization Dependence of Excess Loss of Amorphous Coating Supermirror in Optical Region for Cavity Ringdown Spectroscopy
• Non canonical polarizations of Gravitational Waves
• Deep searches for X-ray pulsations from Scorpius X-1 and Cygnus X-2 in support of continuous gravitational wave searches
• Exploring the Link between Fast Radio Burst and Binary Neutron Star Origins with Spaceborne Gravitational Wave Observations
• Analysing one- and two-bit data to reduce memory requirements for F-statistic-based gravitational wave searches
• Design of a tabletop interferometer with quantum amplification
• Search for sub-solar primordial black holes in low mass ratio binaries with LIGO-Virgo O2 data and implications for the primordial black hole dark matter fraction
• Prospects for detecting and localizing short-duration transient gravitational waves from glitching neutron stars without electromagnetic counterparts
• Impact of correlated seismic and correlated Newtonian noise on the Einstein Telescope
• General Relativistic Stability and Gravitational Wave Content of Rotating Triaxial Neutron Stars
• Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors
• Redshift factor and the small mass-ratio limit in binary black hole simulations
• Parameter estimation for space-based gravitational wave detectors with ringdown signals
• Comparing Bayes factors and hierarchical inference for testing general relativity with gravitational waves
• Constraining runaway dilaton models using joint gravitational-wave and electromagnetic observations
• Gravitational Waves by Perturbation of a Slowly Rotating Thin-Shell Wormhole
• Energetics and scattering of gravitational two-body systems at fourth post-Minkowskian order
• Deep Residual Error and Bag-of-Tricks Learning for Gravitational Wave Surrogate Modeling
• Characterization of merging black holes with two precessing spins
• Incorporating a radiative hydrodynamics scheme in the numerical-relativity code BAM
• Terrestrial Laser Interferometers
• Prospects for distinguishing dynamical tides in inspiralling binary neutron stars with third generation gravitational-wave detectors
• An Order Statistics Post-Mortem on LIGO-Virgo GWTC-2 Events Analysed with Nested Sampling
• Constraining the Time of Gravitational Wave Emission from Core-Collapse Supernovae
• Differentiating between sharp and smoother phase transitions in neutron stars
• Gravitational-wave asteroseismology with f-modes from neutron star binaries at the merger phase
• Gravitational-Wave Geodesy: Defining False Alarm Probabilities with Respect to Correlated Noise
• Precision optomechanics for geometrically modematched Fabry-Perot cavities in ALPS II
• A machine learning algorithm for minute-long Burst searches
• Dynamical double black holes and their host cluster properties
• Probing neutron stars with the full pre-merger and post-merger gravitational wave signal from binary coalescences
• Using machine learning to auto-tune chi-squared tests for gravitational wave searches
• Detectability of a spatial correlation between stellar-mass black hole mergers and Active Galactic Nuclei in the Local Universe
• Modelling the formation of the first two neutron star-black hole mergers, GW200105 and GW200115: metallicity, chirp masses and merger remnant spins
• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations II: Double Compact Object Rates and Properties
• Distinguishing between dark-matter interactions with gravitational-wave detectors
• Cosmology with Love: Measuring the Hubble constant using neutron star universal relations
• Null-stream-based Bayesian Unmodeled Framework to Probe Generic Gravitational-wave Polarizations
• Multi-messenger parameter inference of gravitational-wave and electromagnetic observations of white dwarf binaries
• EFPE: Efficient fully precessing eccentric gravitational waveforms for binaries with long inspirals
• Gravitational background from dynamical binaries and detectability with 2G detectors
• Waveforms and fluxes: Towards a self-consistent effective one body waveform model for nonprecessing, coalescing black-hole binaries for third generation detectors
• Correlation analysis for isotropic stochastic gravitational wave backgrounds with maximally allowed polarization degrees
• Testing gravity with the two-body problem
• The nuclear matter density functional under the nucleonic hypothesis
• Proposed large scale monolithic fused silica mirror suspension for 3rd generation gravitational wave detectors
• Multimodal analysis of Gravitational Wave signals and Gamma-Ray Bursts from binary neutron star mergers
• Gravitational Wave Gastronomy
• Joint Analysis Method on Gravitational Waves and Low-Energy Neutrinos to Detect Core-Collapse Supernovae
• $\kappa$-General-Relativity II: An Astrophysical Observable from a 2-Body system
• Observation of an Optical Spring in a Robustly Controlled Signal-Recycled Michelson Interferometer
• Enhancing gravitational-wave detection: a machine learning pipeline combination approach with robust uncertainty quantification
• On Validating Angular Power Spectral Models for the Stochastic Gravitational-Wave Background Without Distributional Assumptions
• Source Confusion of Massive Black Hole Binaries for the Taiji Mission
• A Carillon of Black Holes
• Multi-detector characterization of gravitational-wave burst tensor polarizations with the BayesWave algorithm
• Initial acquisition requirements for optical cavities in the space gravitational wave antennae DECIGO and B-DECIGO
• Applying higher-modes consistency test on GW190814 : lessons on no-hair theorem, nature of the secondary compact object and waveform modeling
• Measuring spin precession from massive black hole binaries with gravitational waves: insights from time-domain signal morphology
• Unified nonparametric equation-of-state inference from the neutron-star crust to perturbative-QCD densities
• Scalar-Induced Gravitational Waves in Palatini $f(R)$ Gravity
• Extending the micro-Hertz detection horizons via orbital resonance effect for geocentric gravitational wave antennas
• Assessment of normalizing flows for parameter estimation on time-frequency representations of gravitational-wave data
• Capability for detection of GW190521-like binary black holes with TianQin
• Impact of Detector Calibration Accuracy on Black Hole Spectroscopy
• MatBYIB: A Matlab-based code for Bayesian inference of extreme mass-ratio inspiral binary with arbitrary eccentricity
• Waveform model for the $(\ell =2,m=0)$ spherical harmonic and the displacement memory contribution from precessing binary black holes
• Normal Approximate Likelihoods to Gravitational Wave Events
• Discrimination of metric theories
• Probing the peak of star formation with the stochastic background of binary black hole mergers
• On the ease of excitation of black hole ringing: Quantifying the importance of overtones by the excitation factors
• Detecting stochastic gravitational wave background from cosmic strings with next-generation detector networks: Component separation based on a multi-source astrophysical foreground noise model
• Phase Diffusion of Light Immersed In Quantum Tides: Open Quantum System Approach
• Detection of the stochastic gravitational wave background with the space-borne gravitational-wave detector network
• Identification of Noise-Associated Glitches in KAGRA O3GK with Hveto
• Gravitational wave optical counterpart searching based on GRAWITA and DLT40 project during LIGO O2 run
• Crystal Eye: all sky MeV monitor with high precision real-time localization
• LigoDV-web: Providing easy, secure and universal access to a large distributed scientific data store for the LIGO Scientific Collaboration
• Circulating pulse cavity enhancement as a method for extreme momentum transfer atom interferometry
• $e^{+}{e}^{-}$ annihilation on the stochastic background of primordial gravitational waves with BKP18
• Gravitational Waves from Gauge Quanta Produced during Inflation
• Reducing suspension control noise with interferometric sensors -- an experimental concept
• SOAR/Goodman Spectroscopic Assessment of Candidate Counterparts of the LIGO-Virgo Event GW190814
• Examining the Gap in the Chirp Mass Distribution of Binary Black Holes
• Model-agnostic gravitational-wave background characterization algorithm
• Constraints and detection capabilities of GW polarizations with space-based detectors in different TDI combinations
• Multi-scale optimal control for Einstein Telescope active seismic isolation
• Applicability of multi-component study on Bayesian searches for targeted anisotropic stochastic gravitational-wave background
• Finding Fast Transients in Real Time Using Novel Light Curve Analysis Algorithm
• Probing missing physics from inspiralling compact binaries via time-frequency tracks
• A New Framework to Detect Multi-Messenger Signals from Bright Sporadic Stochastic Gravitational Wave Background
• Early Warning From Eccentric Compact Binaries: Template Initialization And Sub-dominant Mode Effects
• Lightweight posterior construction for gravitational-wave catalogs with the Kolmogorov-Arnold network
• Using tunable coherence for reaching micrometer coherence lengths and suppressing stray light in a power-recycled Michelson interferometer
• Time-dependent deflection reconstruction: new technique to search for gravitational waves with the cosmic microwave background
• Persistence of post-Newtonian amplitude structure in binary black hole mergers
• Where are Gaia's small black holes?
• Effect of the cosmological parameters on gravitational waves: general analysis
• The DeepFMKit Python package: A toolbox for simulating and analyzing deep frequency modulation interferometers
• Astrophysical or Terrestrial: Machine learning classification of gravitational-wave candidates using multiple-search information
• Thermal noise in complex systems
• Probing the Purely Ingoing Nature of the Black-hole Event Horizon
• Prospects for detecting asteroid-mass primordial black holes in extreme mass-ratio inspirals with continuous gravitational waves
• Operating Gravitational Wave Detectors far from equilibrium
• Demonstration of tilt sensing using a homodyne quadrature interferometric translational sensor
• GEMINI: The First Underground Testbed for Seismic Isolation and Interplatform Control in Next-Generation Gravitational-Wave Detectors
• Aspects of astrophysical particle production and beyond the Standard Model phenomenology
• Uncertainty in predicting the stochastic gravitational wave background from compact binary coalescences
• Extracting the orbital axis from gravitational waves of precessing binary systems
• Constraining the gravitational-wave emission of core-collapse supernovae with ground-based detectors
• Impact of facility timing and coordination for next-generation gravitational-wave detectors
• True and apparent motion of optomechanical resonators, with applications to feedback cooling of gravitational wave detector test masses
• APRIL: Auxiliary Physically-Redundant Information in Loss -- A physics-informed framework for parameter estimation with a gravitational-wave case study
• Enhancing the significance of astrophysical events with multimessenger coincidences
• Beyond general relativity: gravitational waves in non-minimally coupled theories
• Assessing the performance of future space-based detectors: Astrophysical foregrounds and individual sources
• Global time-frequency search for stellar-mass binary black holes in LISA
• Distinguishing between Black Holes and Neutron Stars within a Population of Weak Tidal Measurements
• The Missing Multipole Problem: Investigating biases from model starting frequency in gravitational-wave analyses
• Upper-limit on the Advanced Virgo output mode cleaner cavity length noise
• Comparative Analysis of Thermal Models for Test Masses in Next-Generation Gravitational Wave Interferometers
• Calculating the static gravitational two-body potential to fifth post-Newtonian order with Feynman diagrams
• Building A Field: The Future of Astronomy with Gravitational Waves, A State of The Profession Consideration for Astro2020
• Prospects for Neutrino Observation and Mass Measurement from Binary Neutron Star Mergers
• Searching Stochastic Gravitational Wave Background Landscape Across Frequency Bands
• Toward a Unified Understanding of the Dense Matter Equation of State
• Search for planetary-mass ultra-compact binaries using data from the first part of the LIGO--Virgo--KAGRA fourth observing run
• Characterizing Binary Black Hole Subpopulations in GWTC-4 with Binned Gaussian Processes: On the Origins of the $35M_{\odot }$ Peak
• Performance of multi-detector hybrid statistic in targeted compact binary coalescence search
• Apparatus to Measure Optical Scatter of Coatings Versus Annealing Temperature
• Effects of local cosmic inhomogeneities on the gravitational wave event rate
• GFH-v2 Pipeline for Searches of Long-Transient Gravitational Waves from Newborn Magnetars
• BinaryGFH-v2: Improved method to search for gravitational waves from sub-solar-mass, ultra-compact binaries using the Generalized Frequency-Hough Transform
• Gravitational waves from spinning neutron stars as not-quite-standard sirens
• Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing?
• Wave Front Sensing demodulated at the difference frequency between two phase-modulation sidebands in a compound interferometer configuration for a gravitational-wave detector
• Extract non-Gaussian Features in Gravitational Wave Observation Data Using Self-Supervised Learning
• In situ substrate birefringence characterization in gravitational wave detectors using a heterodyne polarimetry method
• Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition
• Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter
• Enhancing online estimation of CBC parameters with the low-latency MBTA analysis
• Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses
• The Sequential Monte Carlo goes NUTS: Boosting Gravitational-Wave Inference
• Plunge-Merger-Ringdown Tests of General Relativity with GW250114
• Determination of the light exposure on the photodiodes of a new instrumented baffle for the Virgo input mode cleaner end-mirror
• Population Properties of Binary Black Holes with Eccentricity
• Searching for gravitational waves from compact binary mergers powering long gamma-ray bursts during LIGO-Virgo-KAGRA's O3 run
• Identifying Host Galaxies of Binary Black Hole Mergers with Next-Generation Gravitational Wave Detector Networks
• Cordierite-based optical resonators with extremely low thermal expansion
• Mock Catalogs of Strongly Lensed Gravitational Waves via A Halo Model Approach with Ground-based Detectors
• Narrowband searches for continuous gravitational waves from known pulsars in the first two parts of the fourth LIGO--Virgo--KAGRA observing run
• Las Cumbres Observatory Gravitational-Wave Follow-up in the Third and Fourth Observing Runs: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy
• Joint Detection and Characterization of the Standing Accretion Shock Instability for Core-Collapse Supernovae with cWB XP
• Could the high-mass black holes from gravitational-wave observations be explained by lensing?
• Gravitational-wave astronomy requires population-informed parameter estimation
• Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars
• labrador: A domain-optimized machine-learning tool for gravitational wave inference
• Hierarchical search for compact binary coalescences in the Advanced LIGO's first two observing runs
• Tests of scalar polarizations with multi-messenger events
• Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies
• Direct N-body simulations of rotating and extremely massive Population III star clusters
• No model-independent evidence for a peak in binary black hole spin (mis)alignments
• Binary Black Hole Parameter Estimation with Hybrid CNN-Transformer Neural Networks
• Efficient Evaluation of Gravitational Lensing Amplification Factors: A Deep Learning Framework
• Gravitational-wave standard sirens and application in cosmology
• Constraints on the VHE counterpart of two binary black hole mergers observed by the MAGIC and CTAO LST-1 telescopes
• Testing f(R) gravity using gravitational-wave signals from binary mergers
• Unveiling gravitational waves from core-collapse supernovae with MUSE