GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run

Abstract

The third Gravitational-Wave Transient Catalog (GWTC-3) describes signals detected with Advanced LIGO and Advanced Virgo up to the end of their third observing run. Updating the previous GWTC-2.1, we present candidate gravitational waves from compact binary coalescences during the second half of the third observing run (O3b) between 1 November 2019, 15:00 UTC and 27 March 2020, 17:00 UTC. There are 35 compact binary coalescence candidates identified by at least one of our search algorithms with a probability of astrophysical origin $p_{\mathrm{astro}}>0.5$. Of these, 18 were previously reported as low-latency public alerts, and 17 are reported here for the first time. Based upon estimates for the component masses, our O3b candidates with $p_{\mathrm{astro}}>0.5$ are consistent with gravitational-wave signals from binary black holes or neutron star-black hole binaries, and we identify none from binary neutron stars. However, from the gravitational-wave data alone, we are not able to measure matter effects that distinguish whether the binary components are neutron stars or black holes. The range of inferred component masses is similar to that found with previous catalogs, but the O3b candidates include the first confident observations of neutron star-black hole binaries. Including the 35 candidates from O3b in addition to those from GWTC-2.1, GWTC-3 contains 90 candidates found by our analysis with $p_{\mathrm{astro}}>0.5$ across the first three observing runs. These observations of compact binary coalescences present an unprecedented view of the properties of black holes and neutron stars.

88 pages (10 pages author list, 31 pages main text, 1 page acknowledgements, 24 pages appendices, 22 pages bibliography), 17 figures, 16 tables. Update to match version to be published in Physical Review X. Data products available from https://gwosc.org/GWTC-3/

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• A Galaxy-Targeted Search for the Optical Counterpart of the Candidate NS-BH Merger S190814bv with Magellan
• Characterising Transient Noise in the LIGO Detectors
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• 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
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• Digging the population of compact binary mergers out of the noise
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• Hybrid geometric-random template placement algorithm for gravitational wave searches from compact binary coalescences
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• Swift-XRT follow-up of gravitational wave triggers during the third aLIGO/Virgo observing run
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• Black-hole spectroscopy: quasinormal modes, ringdown stability and the pseudospectrum
• Impact of ringdown higher-order modes on black-hole mergers in dense environments: the scalar field case, detectability and parameter biases
• Accretion disks and relativistic line broadening in boson star spacetimes
• Testing the nature of gravitational wave propagation using dark sirens and galaxy catalogues
• Continuous Gravitational Waves: A New Window to Look for Heavy Non-annihilating Dark Matter
• Formation of Merging Stellar-Mass Black Hole Binaries by Gravitational Wave Emission in Active Galactic Nucleus Disks
• Parity violation in gravitational waves and observational bounds from third-generation detectors
• Spin Hall effects in the sky
• Bondi-Hoyle-Lyttleton accretion onto a rotating black hole with ultralight scalar hair
• Characterization of Laser Systems at 1550 nm Wavelength for Future Gravitational Wave Detectors
• Probing modified gravitational-wave propagation with extreme mass-ratio inspirals
• Rotating Love: The dynamical tides of spinning Newtonian stars
• Rotating black holes experience dynamical tides
• Constraining extended cosmologies with GW$\times$LSS cross-correlations
• Dark Black Holes in the Mass Gap
• Perturbing the vortex: quasinormal and quasibound spectra of rotating acoustic geometries
• Pseudospectrum of rotating analog black holes
• Parametrized spin-precessing inspiral-merger-ringdown waveform model for tests of general relativity
• Multi-messenger Gravitational Lensing
• Primordial black holes: constraints, potential evidence and prospects
• Defining eccentricity for spin-precessing binaries
• Adding equatorial-asymmetric effects for spin-precessing binaries into the SEOBNRv5PHM waveform model
• A rapid channel for the collisional formation and gravitational wave driven mergers of supermassive black hole seeds at high redshift
• The birth mass function of neutron stars
• Stellar-mass black-hole binaries in LISA: characteristics and complementarity with current-generation interferometers
• Incorporation of model accuracy in gravitational wave Bayesian inference
• General relativistic magnetized Bondi-Hoyle-Lyttleton accretion with a spin-field misalignment: Jet nutation, polarity reversals, and Magnus drag
• Binary neutron star mergers as the source of the highest energy cosmic rays
• Multi-messenger Probes of Asteroid Mass Primordial Black Holes: Superradiance Spectroscopy, Hawking Radiation, and Microlensing
• Fast marginalization algorithm for optimizing gravitational wave detection, parameter estimation and sky localization
• Consistent eccentricities for gravitational wave astronomy: Resolving discrepancies between astrophysical simulations and waveform models
• Primordial Black Holes and Scalar-induced Gravitational Waves in Radiative Hybrid Inflation
• Causality and quasi-normal modes in the GREFT
• Correlations for an anisotropic polarized stochastic gravitational wave background in pulsar timing arrays
• Search for eccentric NSBH and BNS mergers in the third observing run of Advanced LIGO and Virgo
• Gravitational-wave constraints on scalar-tensor gravity from a neutron star and black-hole binary GW200115
• Analysis of GWTC-3 with fully precessing numerical relativity surrogate models
• Enabling multi-messenger astronomy with continuous gravitational waves: early warning and sky localization of binary neutron stars in Einstein Telescope
• Constraints on cosmologically coupled black holes from gravitational wave observations and minimal formation mass
• Measuring the Hubble Constant Using Strongly Lensed Gravitational Wave Signals
• Revisiting the Affleck-Dine mechanism for primordial black hole formation
• Signatures of dark and baryonic structures on weakly lensed gravitational waves
• First eccentric inspiral-merger-ringdown analysis of neutron star-black hole mergers
• Multipole expansion at the level of the action in $d$-dimensions
• Mimicking Mergers: Mistaking Black Hole Captures as Mergers
• A geometric template bank for the detection of spinning low-mass compact binaries with moderate orbital eccentricity
• Linear vs. nonlinear modeling of black hole ringdowns
• Constraints on charged black holes from merger-ringdown signals in GWTC-3 and prospects for the Einstein Telescope
• The Impact of Spin in Compact Binary Foreground Subtraction for Estimating the Residual Stochastic Gravitational-wave Background in Ground-based Detectors
• Applying the Viterbi Algorithm to Planetary-Mass Black Hole Searches
• Primordial Black Hole Merger Rate in $f(R)$ Gravity
• Identifying glitches near gravitational-wave signals from compact binary coalescences using the Q-transform
• Search for gravitational waves emitted from SN 2023ixf
• Improving the Cosmological Constraints by Inferring the Formation Channel of Extreme-mass-ratio Inspirals
• Improved inspiral-merger-ringdown model for BBHs on elliptical orbits
• Gravitational Waves in Chern-Simons-Gauss-Bonnet Gravity
• Possible binary neutron star merger history of the primary of GW230529
• Gravitational wave memory of compact binary coalescence in the presence of matter effects
• Merging black holes with Cauchy-characteristic matching: Computation of late-time tails
• Anatomy of parameter-estimation biases in overlapping gravitational-wave signals
• Dark Stars and Gravitational Waves: Topical Review
• Dynamical quasinormal mode excitation
• Search for neutrino counterparts to the gravitational wave sources from LIGO/Virgo O3 run with the ANTARES detector
• A waveform model for the missing quadrupole mode from black hole coalescence: memory effect and ringdown of the $(\ell =2,m=0)$ spherical harmonic
• The clustering of dark sirens' invisible host galaxies
• Electromagnetic fields in compact binaries: post-Newtonian wave generation and application to double white dwarfs systems
• Exploring field-evolution and dynamical-capture coalescing binary black holes in GWTC-3
• Long-term stable nonlinear evolutions of ultracompact black-hole mimickers
• SLICK: Strong Lensing Identification of Candidates Kindred in gravitational wave data
• Impact of dark matter spikes on the merger rates of Primordial Black Holes
• Angular bispectrum and trispectrum of scalar-induced gravitational waves: all contributions from primordial non-Gaussianity $f_{\mathrm{NL}}$ and $g_{\mathrm{NL}}$
• Self-Gravity Effects of Ultralight Boson Clouds Formed by Black Hole Superradiance
• Influence of dark matter equation of state on the axial gravitational ringing of supermassive black holes
• Premerger detection of massive black hole binaries using deep learning
• The Irrelevance of Primordial Black Hole Clustering in the LVK mass range
• Prompt sky localization of compact binary sources using a meshfree approximation
• Frequency-dependent squeezing for gravitational-wave detection through quantum teleportation
• On spin optics for gravitational waves lensed by a rotating object
• Gravitational waves from neutron-star mountains
• Testing eccentric corrections to the radiation-reaction force in the test-mass limit of effective-one-body models
• Post-adiabatic waveform-generation framework for asymmetric precessing binaries
• Quasinormal modes of slowly-spinning horizonless compact objects
• Gravitational-wave background in bouncing models from semi-classical, quantum and string gravity
• A robust cosmic standard ruler from the cross-correlations of galaxies and dark sirens
• Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
• Revealing the ${\chi }_{\mathrm{eff}}$-$q$ Correlation among Coalescing Binary Black Holes and Tentative Evidence for AGN-driven Hierarchical Mergers
• Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes
• Reconstructing the Hubble parameter with future Gravitational Wave missions using Machine Learning
• Search for a gravitational wave background from primordial black hole binaries using data from the first three LIGO-Virgo-KAGRA observing runs
• Calibrating signal-to-noise ratio detection thresholds using gravitational-wave catalogs
• Black hole perturbations in higher-order scalar-tensor theories: initial value problem and dynamical stability
• Disentangling the Black Hole Mass Spectrum with Photometric Microlensing Surveys
• Gravitational radiation from inspiralling compact binaries to N${}^3$LO in the Effective Field Theory approach
• The implications of stochastic gas torques for asymmetric binaries in the LISA band
• Indication for a compact object next to a LIGO-Virgo binary black hole merger
• Strong Field Scattering of Black Holes: Assessing Resummation Strategies
• Intermediate-mass black hole binary parameter estimation with next-generation ground-based detector networks
• Recipes for computing radiation from a Kerr black hole using a generalized Sasaki-Nakamura formalism: Homogeneous solutions
• Neural post-Einsteinian framework for efficient theory-agnostic tests of general relativity with gravitational waves
• Parametrized tests of general relativity using eccentric compact binaries
• Evidence for a strong 19.5 Hz flux oscillation in Swift BAT and Fermi GBM gamma-ray data from GRB 211211A
• Gravitational radiations from periodic orbits around Einstein-Æther black holes
• Gravitational-wave cosmology with dark sirens: state of the art and perspectives for 3G detectors
• Accounting for numerical-relativity calibration uncertainty in gravitational-wave modeling and inference
• Hydrodynamic simulations of black hole evolution in AGN discs I: orbital alignment of highly inclined satellites
• Gravitational-wave imprints of non-convex dynamics in binary neutron star mergers
• Constraining the impact of standard model phase transitions on primordial black holes
• Rapid inference and comparison of gravitational-wave population models with neural variational posteriors
• Black Hole Supernovae, their Equation of State Dependence and Ejecta Composition
• Evolution of a black hole cluster in full general relativity
• Validating Prior-informed Fisher-matrix Analyses against GWTC Data
• Visualizing convolutional neural network for classifying gravitational waves from core-collapse supernovae
• Neural network time-series classifiers for gravitational-wave searches in single-detector periods
• Fast Likelihood-free Reconstruction of Gravitational Wave Backgrounds
• GWDALI: A Fisher-matrix based software for gravitational wave parameter-estimation beyond Gaussian approximation
• Matched filtering for gravitational wave detection without template bank driven by deep learning template prediction model bank
• Exploring Black Hole Mimickers: Electromagnetic and Gravitational Signatures of AdS Black Shells
• Structure and Skewness of the Effective Inspiral Spin Distribution of Binary Black Hole Mergers
• Implications of GWTC-3 on primordial black holes from vacuum bubbles
• Comparative study of 1D and 2D convolutional neural network models with attribution analysis for gravitational wave detection from compact binary coalescences
• Rapid binary mass transfer: Circumbinary outflows and angular momentum losses
• Gravitational wave triggered searches for high-energy neutrinos from binary neutron star mergers: prospects for next generation detectors
• Formation of GW230529 from Isolated Binary Evolution
• Quasinormal Modes in Modified Gravity using Physics-Informed Neural Networks
• Enhancing interferometry using weak value amplification with real weak values
• Do both black holes spin in merging binaries? Evidence from GWTC-4 and astrophysical implications
• Search for continuous gravitational wave signals from luminous dark photon superradiance clouds with LVK O3 observations
• Quick recipes for gravitational-wave selection effects
• Noise in the LIGO Livingston Gravitational Wave Observatory due to Trains
• Bounds on tidal charges from gravitational-wave ringdown observations
• Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning
• Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
• Optimizing post-Newtonian parameters and fixing the BMS frame for numerical-relativity waveform hybridizations
• Parameter estimation of microlensed gravitational waves with Conditional Variational Autoencoders
• Tidal effects in gravitational waves from neutron stars in scalar-tensor theories of gravity
• Simulating binary black hole mergers using discontinuous Galerkin methods
• Probing the Unstable Spectrum of Schwarzschild-like Black Holes
• Impact of anti-symmetric contributions to signal multipoles in the measurement of black-hole spins
• Tidal Forces in Majumdar-Papapetrou Spacetimes
• Probing Spin-Induced Quadrupole Moments in Precessing Compact Binaries
• Searching for gravitational-wave bursts with space-borne detectors
• Primordial Black Hole-Neutron Star Merger Rate in Modified Gravity
• Simulations of Ellipsoidal Primordial Black Hole Formation
• Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Nucleonic models
• Scalable data-analysis framework for long-duration gravitational waves from compact binaries using short Fourier transforms
• Robust inference of gravitational wave source parameters in the presence of noise transients using normalizing flows
• Axial perturbations of hairy black holes in generalised scalar-tensor theories
• A fully precessing higher-mode surrogate model of effective-one-body waveforms
• Modeling lunar response to gravitational waves using normal-mode approach and tidal forcing
• Eccentricity enables the earliest warning and localization of gravitational waves with ground-based detectors
• Mind the step: On the frequency-domain analysis of gravitational-wave memory waveforms
• Real modes and null memory contributions in effective-one-body models
• Constraining ultra slow roll inflation using cosmological datasets
• Testing the nature of GW200105 by probing the frequency evolution of eccentricity
• Quantum precision limits of displacement noise free interferometers
• Improved parametrized test of general relativity using the IMRPhenomX waveform family: Including higher harmonics and precession
• Probe and Prejudice: Classification of compact objects and model comparison using EOS knowledge
• Efficient Stochastic Template Bank using Inner Product Inequalities
• Multi-spectral Sirens: Gravitational-wave Cosmology with (Multi-) Sub-populations of Binary Black Holes
• Quasinormal modes of hairy black holes in shift-symmetric theories
• No evidence for a dip in the binary black hole mass spectrum
• Constraints on Inflation with Null Energy Condition Violation from Advanced LIGO and Advanced Virgo's First Three Observing Runs
• An interference-based method for the detection of strongly lensed gravitational waves
• Secondary spins of extreme mass ratio inspirals: A probe to the formation channels
• Parameter Estimation with Nonstationary Noise in Gravitational-wave Data
• A Mid-Thirties Crisis: Dissecting the Properties of Gravitational Wave Sources Near the 35 Solar Mass Peak
• Gravitational Wave Measurement in the Mid-Band with Atom Interferometers
• Gravitational Radiation from Eccentric Binary Black Hole System in Dynamical Chern-Simons Gravity
• Second MAYA Catalog of Binary Black Hole Numerical Relativity Waveforms
• Peaking into the abyss: Characterizing the merger of equatorial-eccentric-geodesic plunges in rotating black holes
• GPU-accelerated LISA parameter estimation with full time domain response
• Primordial Black Holes without fine-tuning from a light stochastic spectator field
• SAGUARO: Time-domain Infrastructure for the Fourth Gravitational-wave Observing Run and Beyond
• Massive neutron stars as mass gap candidates: Exploring equation of state and magnetic field
• Impact of overlapping signals on parameterized post-Newtonian coefficients in tests of gravity
• Template bank to search for exotic gravitational wave signals from astrophysical compact binaries
• McFACTS II: Mass Ratio--Effective Spin Relationship of Black Hole Mergers in the AGN Channel
• Reanalyzing the ringdown signal of GW150914 using the F-statistic method
• Models of cosmological black holes
• Inference of multi-channel r-process element enrichment in the Milky Way using binary neutron star merger observations
• Probing dark-matter effects with gravitational waves using the parameterized post-Einsteinian framework
• Cosmology and nuclear-physics implications of a subsolar gravitational-wave event
• Determining the Hubble Constant with AGN-assisted Black Hole Mergers
• A neural network emulator of the Advanced LIGO and Advanced Virgo selection function
• Improving cosmological reach of a gravitational wave observatory using Deep Loop Shaping
• Numerical relativity surrogate models for exotic compact objects: the case of head-on mergers of equal-mass Proca stars
• Primordial Black Holes and Scalar-induced Gravitational Waves in Sneutrino Hybrid Inflation
• Neutrino spin and flavor oscillations in gravitational fields
• Lensing and wave optics in the strong field of a black hole
• Bayesian real-time classification of multi-messenger electromagnetic and gravitational-wave observations
• $\mu$-GLANCE: A Novel Technique to Detect Chromatically and Achromatically Lensed Gravitational Wave Signals
• Resonant excitation of eccentricity in spherical extreme-mass-ratio inspirals
• Can we discern millilensed gravitational-wave signals from signals produced by precessing binary black holes with ground-based detectors?
• Muffled Murmurs: Environmental effects in the LISA stochastic signal from stellar-mass black hole binaries
• Fundamental Physics and Cosmology with TianQin
• Polarization modes of gravitational waves in general Einstein-vector theory
• Toward a test of Gaussianity of a gravitational wave background
• Deep learning to detect gravitational waves from binary close encounters: Fast parameter estimation using normalizing flows
• The Gravitational-wave Optical Transient Observer (GOTO)
• Spin effects in the phasing formula of eccentric compact binary inspirals up to the third post-Newtonian order
• Systematic biases from ignoring environmental tidal effects in gravitational wave observations
• Constraining string cosmology with the gravitational-wave background using the NANOGrav 15-year data set
• Probing Interacting Dark Sector with the next generation of gravitational-wave detectors
• Gravitational wave ringdown analysis using the $\mathcal{F}$-statistic
• Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object
• Waveform systematics in identifying strongly gravitationally lensed gravitational waves: Posterior overlap method
• Pinpointing coalescing binary neutron star sources with the IGWN, including LIGO-Aundha
• Gravitational Wave Searches for Post-Merger Remnants of GW170817 and GW190425
• Mass and tidal parameter extraction from gravitational waves of binary neutron stars mergers using deep learning
• Assessing the stability of ultracompact spinning boson stars with nonlinear evolutions
• XKN: a Semi-analytic Framework for the Modelling of Kilonovae
• Ringdowns for black holes with scalar hair: the large mass case
• Highly accurate simulations of asymmetric black-hole scattering and cross validation of effective-one-body models
• Sensors and Actuators for the Advanced LIGO+ Upgrade
• Multidimensional hierarchical tests of general relativity with gravitational waves
• Confronting general relativity with principal component analysis: Simulations and results from GWTC-3 events
• False positives for gravitational lensing: the gravitational-wave perspective
• Evidence of a fraction of LIGO/Virgo/KAGRA events coming from active galactic nuclei
• Impact of higher harmonics of gravitational radiation on the population inference of binary black holes
• Comparison between time-domain and frequency-domain Bayesian inferences to inspiral-merger-ringdown gravitational-wave signals
• Primordial black-hole formation and heavy r-process element synthesis from the cosmological QCD transition. Two aspects of an inhomogeneous early Universe
• Transition-to-plunge self-force waveforms with a spinning primary
• Constraints on Brans-Dicke gravity from neutron star-black hole merger events using higher harmonics
• Reconstructing parametric gravitational-wave population fits from non-parametric results without refitting the data
• Probing dark matter halo profiles with multi-band observations of gravitational waves
• Piecewise frequency model for searches for long-transient gravitational waves from young neutron stars
• Bounds on the charge of the graviton using gravitational wave observations
• Primordial Black-Hole-Based Pathways to Little Red Dots
• Gravitational-Wave Parameter Estimation in non-Gaussian noise using Score-Based Likelihood Characterization
• Modified gravitational wave propagations in linearized gravity with Lorentz and diffeomorphism violations and their gravitational wave constraints
• Hair is complicated: Gravitational waves from stable and unstable boson-star mergers
• Magnification and evolution bias of transient sources: GWs and SNIa
• Constraints on the Pre-Big Bang scenario from a cosmological interpretation of the NANOGrav data
• Multi-messenger astronomy with a Southern-Hemisphere gravitational-wave observatory
• Nature of phase transitions and metastability in scalar-tensor theories
• Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset
• The curvature dependence of gravitational-wave tests of General Relativity
• Unveiling the solution to the final-parsec problem by combining milli-Hertz gravitational-wave observation and AGN survey
• Convolutional Neural Networks for signal detection in real LIGO data
• Constraints on peculiar velocity distribution of binary black holes using gravitational waves with GWTC-3
• Octupolar test of general relativity
• Implementation of a generalized precession parameter in the RIFT parameter estimation algorithm
• Eccentricity matters: Impact of eccentricity on inferred binary black hole populations
• Recovering Injected Astrophysics from the LISA Galactic Double White Dwarf Binaries
• Post-Newtonian Dynamics of Spinning Black Hole Binaries in Einstein-Scalar-Gauss-Bonnet Gravity
• Proper Time Observables of General Gravitational Perturbations in Laser Interferometry-based Gravitational Wave Detectors
• Binary dynamics to second post-Newtonian order in scalar-tensor and Einstein-scalar-Gauss-Bonnet gravity from effective field theory
• Borexino's search for low-energy neutrinos associated with gravitational wave events from GWTC-3 database
• Enhancing search pipelines for short gravitational wave transients with Gaussian mixture modelling
• Data-driven extraction, phenomenology and modeling of eccentric harmonics in binary black hole merger waveforms
• LitePIG: A Lite Parameter Inference system for the Gravitational wave in the millihertz band
• Autonomous Disentangling for Spectroscopic Surveys
• High priority targets for transient gravitational waves from glitching pulsars
• Constraining gravitational-wave backgrounds from conversions into photons in the Galactic magnetic field
• Spinning waveforms of scalar radiation in quadratic modified gravity
• Searching for gravitational waves from stellar-mass binary black holes early inspiral
• Complete quasinormal modes of Type-D black holes
• Methodology for constraining ultralight vector bosons with gravitational wave searches targeting merger remnant black holes
• Phenomenological gravitational waveform model of binary black holes incorporating horizon fluxes
• Inferring small neutron star spins with neutron star-black hole mergers
• Parameterized quasinormal frequencies and Hawking radiation for axial gravitational perturbations of a holonomy-corrected black hole
• Extended mass distribution of PBHs during QCD phase transition: SGWB and mini-EMRIs
• Compact object populations over cosmic time II. Compact object merger rates and masses over redshift from varying initial conditions
• Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary
• Compact Binary Merger Rate with Modified Gravity in Dark-Matter Spikes
• Bayesian Search of Massive Scalar Fields from LIGO-Virgo-KAGRA Binaries
• Bayesian inference of neutron star crust properties using an ab initio-benchmarked meta-model
• The large-scale anisotropy and flux (de-)magnification of ultra-high-energy cosmic rays in the Galactic magnetic field
• cDVGAN: One Flexible Model for Multi-class Gravitational Wave Signal and Glitch Generation
• Observable-based reformulation of time-delay interferometry
• Observability of spin precession in the presence of a black-hole remnant kick
• Automated Evaluation of Environmental Coupling for Advanced LIGO Gravitational Wave Detections
• Gravitational waves and galaxies cross-correlations: a forecast on GW biases for future detectors
• Biased parameter inference of eccentric, spin-precessing binary black holes
• Probing charge of compact objects with gravitational microlensing of gravitational waves
• Likelihood for a Network of Gravitational-Wave Detectors with Correlated Noise
• Post-Newtonian expansion of gravitational energy and angular momentum fluxes: inclined spherical orbits about a Kerr black hole
• Binary dynamics from Einstein-Maxwell theory at second post-Newtonian order using effective field theory
• Wavelet-based tools to analyze, filter, and reconstruct transient gravitational-wave signals
• Relevance of Precession for Tests of the Black Hole No Hair Theorems
• Navigating Unknowns: Deep Learning Robustness for Gravitational Wave Signal Reconstruction
• The First Model-Independent Chromatic Microlensing Search: No Evidence in the Gravitational Wave Catalog of LIGO-Virgo-KAGRA
• Which is which? Identification of the two compact objects in gravitational-wave binaries
• Modeling matter(s) in SEOBNRv5THM: Generating fast and accurate effective-one-body waveforms for spin-aligned binary neutron stars
• Validating Sequential Monte Carlo for Gravitational-Wave Inference
• Reconstruction of binary black hole harmonics in LIGO using deep learning
• Binary Neutron Star Merger Search Pipeline Powered by Deep Learning
• No Glitch in the Matrix: Robust Reconstruction of Gravitational Wave Signals Under Noise Artifacts
• New approach to template banks of gravitational waves with higher harmonics: Reducing matched-filtering cost by over an order of magnitude
• The origin channels of hierarchical binary black hole mergers in the LIGO-Virgo-KAGRA O1, O2, and O3 runs
• Reducing controls noise in gravitational wave detectors with interferometric local damping of suspended optics
• Hydrodynamic simulations of black hole evolution in AGN discs II: inclination damping for partially embedded satellites
• Memory of a Random Walk: Astrometric deflections from gravitational wave memory accumulation over cosmological scales
• Displacement-noise-free neutron interferometer for gravitational wave detection using a single Mach-Zehnder configuration
• Eccentricity evolution consistency test to distinguish eccentric gravitational-wave signals from eccentricity mimickers
• Deep-Learning Classification and Parameter Inference of Rotational Core-Collapse Supernovae
• A rapid black hole spin or emission from the plunging region?
• Accelerating Bayesian Sampling for Massive Black Hole Binaries with Prior Constraints from Conditional Variational Autoencoder
• Exploring the Dynamics of General Relativistic Binary-Single and Binary-Binary Encounters of Black Holes
• Frequency contamination from new fundamental fields in black hole ringdowns
• Fast and accurate parameter estimation of high-redshift sources with the Einstein Telescope
• Taming systematics in distance and inclination measurements with gravitational waves: role of the detector network and higher-order modes
• Conservative Dynamics of Relativistic Binaries Beyond Einstein Gravity
• Modeling Gravitational Wave Modes from the Inspiral of Binaries with Arbitrary Eccentricity
• Constraining parity and Lorentz violations in gravity with future ground- and space-based gravitational wave detectors
• Vortices without inflow: bound spectra in horizonless rotational analogs
• Quantum decoherence of gravitational waves
• Cumulative effect of orbital resonances in extreme-mass-ratio inspirals
• Gravitational-wave memory effects in the Damour-Esposito-Farèse extension of Brans-Dicke theory
• Optimizing Neural Network Surrogate Models: Application to Black Hole Merger Remnants
• A Deep Learning Powered Numerical Relativity Surrogate for Binary Black Hole Waveforms
• Field Sources for Wormholes With Multiple Throats/Anti-throats
• Cosmic Cartography II: completing galaxy catalogs for gravitational-wave cosmology
• Post-adiabatic waveforms from extreme mass ratio inspirals in the presence of dark matter
• Direct nonparametric multimessenger constraints on the equation of state of cold dense nuclear matter
• Comparison and application of different post-Newtonian models for inspiralling stellar-mass binary black holes with space-based GW detectors
• Accelerated parameter estimation of supermassive black hole binaries in LISA using a meshfree approximation
• Clock synchronization and light-travel-time estimation for space-based gravitational-wave detectors
• Next-generation global gravitational-wave detector network: Impact of detector orientation on compact binary coalescence and stochastic gravitational-wave background searches
• Measuring the Spin of the Galactic Center Supermassive Black Hole with Two Pulsars
• Method to search for inspiraling planetary-mass ultra-compact binaries using the generalized frequency-Hough transform in LIGO O3a data
• A Sea of Black Holes: Characterizing the LISA Signature for Stellar-Origin Black Hole Binaries
• Forecast Analysis of Astrophysical Stochastic Gravitational Wave Background beyond general relativity: A Case Study on Brans-Dicke Gravity
• Observability of dynamical tides in merging eccentric neutron star binaries
• Prospects of constraining on the polarizations of gravitational waves from binary black holes using space- and ground-based detectors
• Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer
• Search for gravitational waves from eccentric binary black holes with an effective-one-body template
• Where did Heavy Binaries Go? Gravitational-wave Populations Using Delaunay Triangulation with Optimized Complexity
• GW230814: investigation of a loud gravitational-wave signal observed with a single detector
• The LISA forecast on a smooth crossover beyond the Standard Model through the scalar-induced gravitational waves
• Background information: a study on the sensitivity of astrophysical gravitational-wave background searches
• Building a bridge between comparable and extreme mass ratio black hole binaries: a single spin precessing model for the final state
• Analytical model of precessing binaries using post-Newtonian theory in the extreme mass-ratio limit I: General Formalism
• Beyond GWTC-3: Analysing and verifying new gravitational-wave events from community catalogues
• Unbiased estimation of gravitational-wave anisotropies from noisy data
• Can Primordial Black Holes form in the Standard Model ?
• Dynamical Tidal Response of Non-rotating Black Holes: Connecting the MST Formalism and Worldline EFT
• Imprints of massive black-hole binaries on neighbouring decihertz gravitational-wave sources
• Detection of GW200105 with a targeted eccentric search
• Impact of Bayesian Priors on the Inferred Masses of Quasi-Circular Intermediate-Mass Black Hole Binaries
• Novel Deep Learning Approach to Detecting Binary Black Hole Mergers
• Dipole Anisotropy in Gravitational Wave Source Distribution
• Probing cosmic chemical enrichment with next-generation gravitational-wave observatories
• Parameter estimation of protoneutron stars from gravitational wave signals using the Hilbert-Huang transform
• Seeking Spinning Subpopulations of Black Hole Binaries via Iterative Density Estimation
• Waging a Campaign: Results from an Injection-Recovery Study involving 35 numerical Relativity Simulations and three Waveform Models
• Reconstructing the LISA massive black hole binary population via iterative kernel density estimation
• The directional isotropy of LIGO-Virgo binaries
• Response of a Kerr black hole to a generic tidal perturbation
• Confronting recent light compact star observations with color-flavor locked quark matter
• Accelerated inference of binary black-hole populations from the stochastic gravitational-wave background
• Eccentric mergers of binary Proca stars
• Hawking Radiation Signatures from Primordial Black Holes Transiting the Inner Solar System: Prospects for Detection
• UniMAP: Model-free detection of unclassified noise transients in LIGO-Virgo data using the Temporal Outlier Factor
• A Bright Future? Prospects for Cosmological Tests of GR with Multimessenger Gravitational Wave Events
• Evolution and detection of vector superradiant instabilities
• 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
• Propagation and lensing of gravitational waves in Palatini $f(\hat{R})$ gravity
• Probing black hole `charge' from the binary black hole inspiral
• Experiment demonstration of tilt-to-length coupling suppression by beam-alignment-mechanism
• Measuring Gravitational Wave Speed and Lorentz Violation with the First Three Gravitational-Wave Catalogs
• Gravitational collapse in Quadratic Gravity
• Limiting the Number of Extra Dimensions with Shortcuts
• DVGAN: Stabilize Wasserstein GAN training for time-domain Gravitational Wave physics
• Identifying and Mitigating Machine Learning Biases for the Gravitational Wave Detection Problem
• Scalar fields around black hole binaries in LIGO-Virgo-KAGRA
• Toward relativistic inspirals into black holes surrounded by matter
• Inferring spin tilts of binary black holes at formation with plus-era gravitational wave detectors
• Gravitational-wave imprints of Kerr--Bertotti--Robinson black holes: frequency blue-shift and waveform dephasing
• A Hubble constant estimation with dark standard sirens and galaxy cluster catalogues
• Effective field theory of coupled dark energy and dark matter
• On the Gauge Invariance of Secondary Gravitational Waves
• Classification uncertainty for transient gravitational-wave noise artefacts with optimised conformal prediction
• Strong lensing of gravitational waves with modified propagation
• Unveiling the electrodynamic nature of spacetime collisions
• PETRA: From the LISA global fit to a catalog of Galactic binaries
• Looking To The Horizon: Probing Evolution in the Black Hole Spectrum With Gravitational Wave Catalogs
• Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements
• Are long gamma-ray bursts progenitors to merging binary black holes?
• Advancing the Effective-One-Body Framework in the Test-Mass Limit
• Potential impact of noise correlation in next-generation gravitational wave detectors
• Profiling stellar environments of gravitational wave sources
• Beware of the running $n_s$ when producing heavy primordial black holes
• Detectability of Gravitational-Wave Memory with LISA: A Bayesian Approach
• Gravitational wave background from primordial black holes in globular clusters
• Parametrized multipolar gravitational waveforms for testing general relativity: Amplitude corrections up to 2PN order
• ROXAS: a new pseudospectral non-linear code for general relativistic oscillations of fast rotating isolated neutron stars
• Searches for neutrino counterparts of gravitational waves from the LIGO/Virgo third observing run with KM3NeT
• Padé metrics for black hole perturbations and light rings
• Lensing Stability and Scattering Phenomena in Anisotropic Black Hole Spacetimes in Plasma
• DeepExtractor: Time-domain reconstruction of signals and glitches in gravitational wave data with deep learning
• Electromagnetic field in a cavity induced by gravitational waves
• Mapping Progenitors of Binary Black Holes and Neutron Stars with Binary Population Synthesis
• What to expect: kilonova light curve predictions via equation of state marginalization
• Primordial black holes and scalar-induced gravitational waves from the polynomial attractor model
• Mapping Parameter Correlations in Spinning Binary Black Hole Mergers
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Obtaining Statistical Significance of Gravitational Wave Signals in Hierarchical Search
• Robust and fast parameter estimation for gravitational waves from binary neutron star merger remnants
• Testing modified gravity with the eccentric neutron star--black hole merger GW200105
• Gravitational-wave signatures of mirror (a)symmetry in binary black hole mergers: measurability and correlation to gravitational-wave recoil
• Optimizing the low-latency localization of gravitational waves
• Magnetic Field Simulation and Correlated Low-Frequency Noise Subtraction for an In-Orbit Demonstrator of Magnetic Measurements
• Exploring the Orbital Alignments of Galactic Close White Dwarf Binaries with LISA
• A Multi-Messenger Search for Exotic Field Emission with a Global Magnetometer Network
• Electromagnetic Follow-up to Gravitational Wave Events with the UltraViolet EXplorer (UVEX)
• The Nature of Gravitational Wave Events with Host Environment Escape Velocities
• Waveform Reconstruction of Core-Collapse Supernova Gravitational Waves with Improved Multisynchrosqueezing Transform
• Ultra High Energy Neutrino Event KM3-230213A as a Signal of Electroweak Vacuum Turbulence in Merging Black Hole Binaries
• Beyond the Long Wavelength Approximation: Next-generation Gravitational-Wave Detectors and Frequency-dependent Antenna Patterns
• Measuring black hole spins with x-ray reflection spectroscopy: A GRMHD outlook
• Bright siren without electromagnetic counterpart by LISA-Taiji-TianQin network
• Impact of Population III stars on the astrophysical gravitational-wave background
• Identification of Strongly Lensed Gravitational Wave Events Using Squeeze-and-Excitation Multilayer Perceptron Data-efficient Image Transformer
• Alternative approach to time-delay interferometry with optical frequency comb
• Primordial Black Holes and Second-order Gravitational Waves in Axion-like Hybrid Inflation
• Epicyclic Frequencies for a Generic Ultracompact Object
• Rates and beaming angles of GRBs associated with compact binary coalescences
• Joint inference for gravitational wave signals and glitches using a data-informed glitch model
• Extending the short gamma-ray burst population from sub-threshold triggers in Fermi/GBM and GECAM data and its implications
• Analytic solutions for the motion of spinning particles near brane-world black hole
• Stellar-Mass Black Holes
• Black hole spectroscopy of collapsing and merging neutron stars
• Analysis and simulations of binary black hole merger spins -- the question of spin-axis tossing at black hole formation
• Quantum Bayesian Inference with Renormalization for Gravitational Waves
• Improved binary black hole searches through better discrimination against noise transients
• Are all models wrong? Falsifying binary formation models in gravitational-wave astronomy
• Leveraging cross-detector parameter consistency measures to enhance sensitivities of gravitational wave searches
• Probing Binary Lens Caustics with Gravitational Waves: A Uniform Approximation Approach
• Strong Field Scattering of Two Black Holes: Exploring Gauge Flexibility
• Black-Hole Cartography
• Waveform models for the gravitational-wave memory effect: Extreme mass-ratio limit and final memory offset
• Confronting primordial black holes with LIGO-Virgo-KAGRA and the Einstein Telescope
• Gravitational lensing aided luminosity distance estimation for compact binary coalescences
• Modulations of Gravitational Waves due to Non-static Gravitational Lenses
• Analyzing black-hole ringdowns with orthonormal modes
• Inferring the spins of merging black holes in the presence of data-quality issues
• Korteweg-de Vries Integrals for Modified Black Hole Potentials: Instabilities and other Questions
• Continuous gravitational waves in the lab: recovering audio signals with a table-top optical microphone
• Inflationary relics from an Ultra-Slow-Roll plateau
• Probing Spin-Orbit Resonances with the Binary Black Hole Population
• I-band photometry of the quiescent black hole X-ray nova GROJ0422+32=V518 Per: modelling of the orbital light curve and estimation of the black hole mass
• Constraining the modified friction in gravitational wave propagation with precessing black hole binaries
• Sensing the vibration of non-reflective surfaces with 10-dB-squeezed-light enhancement
• Robust, Rapid, and Simple Gravitational-wave Parameter Estimation
• Relieving scale disparity in binary black hole simulations
• Accounting for the Known Unknowns: A Parametric Framework to Incorporate Systematic Waveform Errors in Gravitational-Wave Parameter Estimation
• Transient electromagnetic sources can detect solitary black holes in Milky Way galaxy
• Distinguishing dark matter halos with Extreme mass ratio inspirals
• Mergers of hairy black holes: Constraining topological couplings from entropy
• Is GW190521 a gravitational wave echo of wormhole remnant from another universe?
• Binary black hole population inference combining confident and marginal events from the $\mathtt{IAS}\text{-}\mathtt{HM}$ search pipeline
• Joint Inference of Population, Cosmology, and Neutron Star Equation of State from Gravitational Waves of Dark Binary Neutron Stars
• Even-parity stability of hairy black holes in $U(1)$ gauge-invariant scalar-vector-tensor theories
• Bayesian Analysis of Wave-Optics Gravitationally Lensed Massive Black Hole Binaries with Space-Based Gravitational Wave Detector
• 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
• Comparing astrophysical models to gravitational-wave data in the observable space
• Effects of dynamical capture on two equal-mass nonspinning black holes
• Hairy black holes in extended Einstein-Maxwell-scalar theories with magnetic charge and kinetic couplings
• Hierarchical searches for subsolar-mass binaries and the third-generation gravitational wave detector era
• Ergoregion instability in a fluid with vorticity
• Sensitivity forecasts for gravitational-wave detectors to dark matter decaying into gravitons
• On the use of galaxy catalogs in gravitational-wave parameter estimation
• Impact of noise transients on gravitational-wave burst detection efficiency of the BayesWave pipeline with multi-detector networks
• Search for exotic gravitational wave signals beyond general relativity using deep learning
• A pipeline to search for signatures of line-of-sight acceleration in gravitational wave signals produced by compact binary coalescences
• Two-body problem in curved spacetime: exploring gravitational wave transient cases
• Natural polynomials for Kerr quasi-normal modes
• Phase diagrams of quasinormal frequencies for Schwarzschild, Kerr, and Taub-NUT black holes
• One-stop strategy to search for long-duration gravitational-wave signals
• Glitches far from transient gravitational-wave events do not bias inference
• Forecast cosmological constraints from the number counts of Gravitational Waves events
• Inferring jet physics from neutron star - black hole mergers with gravitational waves
• Unmasking noise transients masquerading as intermediate-mass black hole binaries
• Ten years of extreme gravity tests of general theory of relativity with gravitational-wave observations
• Performance of multiple filter-cavity schemes for frequency-dependent squeezing in gravitational-wave detectors
• Detecting Unmodeled, Source-dependent Signals in Gravitational Waves with SCoRe
• Gravitational Lensing in the Kerr Spacetime: An Analytic Approach for Light and High-Frequency Gravitational Waves
• Using t-SNE for characterizing glitches in LIGO detectors
• Testing general relativity with amplitudes of subdominant gravitational-wave modes
• Exploring the anisotropic gravitational wave background from all-sky mock gravitational wave event catalogues
• Phase consistency test to identify type II strongly lensed gravitational wave signals using a single event
• Gravitational lensing inside and outside of a marginally unstable photon sphere in a general, static, spherically symmetric, and asymptotically-flat spacetime in strong deflection limits
• General relativistic hydrodynamics code for dynamical spacetimes with curvilinear coordinates, tabulated equations of state, and neutrino physics
• Self-consistent treatment of thermal effects in neutron-star post-mergers: observational implications for third-generation gravitational-wave detectors
• Massive boson stars: Stability and GW emission in head-on mergers
• Arm-Locking Frequency Noise Suppression for Astronomical Middle-Frequency Interferometric Gravitational Wave Observatory
• An analytical joint prior for effective spins for inference on the spin distribution of binary black holes
• Challenges in Forming Millisecond Pulsar-Black Holes from Isolated Binaries
• Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers
• Multi-parameter Tests of General Relativity Using Bayesian Parameter Estimation with Principal Component Analysis for LISA
• Surrogate modeling of gravitational waves microlensed by spherically symmetric potentials
• Fundamental quantum limits for detecting ultrahigh frequency gravitational waves
• Effect of kick velocity on gravitational wave detection of binary black holes with space- and ground-based detectors
• Population Synthesis of Gravitational Wave Sources
• PycWB: A User-friendly, Modular, and Python-based Framework for Gravitational Wave Unmodelled Search
• Beyond FINDCHIRP: Breaking the memory wall and optimal FFTs for Gravitational-Wave Matched-Filter Searches with Ratio-Filter Dechirping
• Limits on the existence of totally reflective exotic compact objects with current and future gravitational-wave detectors
• Dynamical hair growth in black hole binaries in Einstein-scalar-Gauss-Bonnet gravity
• Overlapping signals in next-generation gravitational wave observatories: A recipe for selecting the best parameter estimation technique
• Search for Higher Harmonic Signals from Close White Dwarf Binaries in the mHz Band
• Weak-Value Amplification for Longitudinal Phase Measurements Approaching the Shot-Noise Limit Characterized by Allan Variance
• Detecting milli-Hz gravitational waves with optical resonators
• Accelerating the time-domain LISA response model with central finite differences and hybridization techniques
• Implications of pulsar timing arrays for Gauss-Bonnet Inflation
• How much spin wandering can continuous gravitational wave search algorithms handle?
• Constraining the environment of compact binary mergers with self-lensing signatures
• Searching for stellar-origin binary black holes in LISA Data Challenge 1b: Yorsh
• Mass function of stellar black holes as revealed by the LIGO-Virgo-KAGRA observations
• Can the Near-Horizon Black Hole Memory be detected through Binary Inspirals?
• Strong-lensing rates of massive black hole binaries in LISA
• Gravitational waves from sub-solar mass primordial black holes
• Neutron star evolution by combining discontinuous Galerkin and finite volume methods
• Detectability of massive binary black holes with sub-mHz gravitational wave missions
• Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr
• Scalable matched-filtering pipeline for gravitational-wave searches of compact binary mergers
• Constraints on gravitational waves from the 2024 Vela pulsar glitch
• Observational bounds on Dark Matter Admixed Neutron Stars from Gravitational Wave Data
• Glitch veto based on unphysical gravitational wave binary inspiral templates
• GWAI: Artificial Intelligence Platform for Enhanced Gravitational Wave Data Analysis
• Significant challenges for astrophysical inference with next-generation gravitational-wave observatories
• Illuminating the Mass Gap Through Deep Optical Constraint on a Neutron Star Merger Candidate S250206dm
• A Gaussian process framework for testing general relativity with gravitational waves
• Neutrinos in colliding neutron stars and black holes
• Improved Binary Black Hole Search Discriminator from the Singular Value Decomposition of Non-Gaussian Noise Transients
• Doppler correlation-driven vetoes for the Frequency Hough analysis in continuous gravitational-wave searches
• Parameter control for binary black hole initial data
• "Industrial-Scale" Black Hole Selection without a Satellite
• A Mass-Shell Model of Compact Binary Coalescence
• Generalized Perturbed Kepler Problem: Gravitational Wave Imprints from Eccentric Compact Binaries
• The first stars
• General Fourier expansion of post-Newtonian binary dynamics based on a quasi-Keplerian framework
• Reducing systematic uncertainties in gravitational-wave population analyses by increasing the detection threshold
• Black hole ringdown spectroscopy of curvature-coupled scalar and pseudoscalar fields
• The Multi-parameter Test of Gravitational Wave Dispersion with Principal Component Analysis
• Radiatively Cooled Binary Mass Transfer: Flow Structure, Luminosities, and L2 Outflows Across Mass Transfer Rates
• A ${\chi }^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences
• Can Big Black Holes Merge with the Smallest Black Holes?
• Binary black holes in the heat of merger
• Gravitational-wave matched filtering on a quantum computer
• Numerical computation of electromagnetically sourced nonlinear tails
• Modeling Relative Peak Times of Gravitational Wave Harmonics
• Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog
• Constraining the abundance of spinning deformed Galactic compact objects with continuous gravitational waves
• 3D Localization of FRB 20190425A for Its Potential Host Galaxy and Implications
• Measurement prospects for the pair-instability mass cutoff with gravitational waves
• The Luminosity of the Darkness: Schechter function in dark sirens
• Flexible Gravitational-Wave Parameter Estimation with Transformers
• Learning and Interpreting Gravitational-Wave Features from CNNs with a Random Forest Approach
• Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia
• Inferring the spin distribution of binary black holes using deep learning
• Prospects for High-Frequency Gravitational-Wave Detection with GEO600
• The impact of precession and higher-order multipoles for gravitational wave cosmological inference
• Perturbations of Einstein--Maxwell--phantom spacetime: Instabilities of charged Ellis--Bronnikov wormholes and quasinormal modes of black holes
• Characterizing Compact-object Binaries in the Lower Mass Gap with Gravitational Waves
• Listening Across the Cosmic Time: Standard Sirens from Ground- and Space-Based Missions in the Next Decade
• Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates
• Bayesian Framework to Follow-up Continuous Gravitational Wave Candidates from Deep Surveys
• Extreme mass ratio inspirals into black holes surrounded by matter: Resonance crossings
• Statistical biases in parametrized searches for gravitational-wave polarizations
• Importance of relativistic pericenter precession in identifying the presence of a third body near eccentric binaries
• Searching for joint neutrino and gravitational wave emission from the environment of Active Galactic Nuclei
• Banks of templates for directed and all-sky narrow-band searches of continuous gravitational waves from spinning neutron stars with several spindowns
• BHaHAHA: A Fast, Robust Apparent Horizon Finder Library for Numerical Relativity
• Black Hole Spin-down in Collapsars in 3D Neutrino Transport GRMHD Simulations
• Outer Solar System spacecraft to probe the $\mu$Hz gravitational wave frontier
• Perturbative Frequency Expansion for Nearly Monochromatic Binary Black Holes Detectable with LISA
• Primordial black holes versus their impersonators at gravitational wave observatories
• Equations of motion for compact binary systems in general relativity: Do they depend on the bodies' internal structure at the third post-Newtonian order?
• Rigorous analytic solution to the gravitational-wave overlapping event rates
• Constraints on High-Frequency Gravitational Waves from Graviton-Photon Conversion in the M87 Galaxy
• Archival Inference for Eccentric Stellar-Mass Binary Black Holes in Space-Based Gravitational Wave Observations
• Expanding the Quantum-Limited Gravitational-Wave Detection Horizon
• Measurement of the Hubble constant using the Dark Energy Survey Year 6 Gold galaxy catalogue and the fourth Gravitational-Wave Transient Catalogue
• Multivariate Time Series Clustering for Environmental State Characterization of Ground-Based Gravitational-Wave Detectors
• Searches for Continuous Gravitational Waves from Supernova Remnants in the first part of the LIGO-Virgo-KAGRA Fourth Observing run
• Gravitational ringdown in the Minimal Theory of Massive Gravity
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• Using overlap of sky localization probability maps for filtering potentially lensed pairs of gravitational-wave signals
• Simulation Study on Constraining GW Propagation Speed by GW and GRB Joint Observation on Binary Neutron Star Mergers
• Astrophysical and Cosmological Relevance of the High-Frequency Features in the Stochastic Gravitational-Wave Background
• Gravitational wave distance estimation using intrinsic signal properties: dark sirens as distance indicators
• 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
• Photon Calibration Performance of KAGRA during the 4th Joint Observing Run (O4)
• Early Warning From Eccentric Compact Binaries: Template Initialization And Sub-dominant Mode Effects
• superB/NRPy: Scalable, Task-Based Numerical Relativity for 3G Gravitational Wave Science
• Probing the peak of star formation with the stochastic background of binary black hole mergers
• Fast Waveform Generation for Gravitational Waves using Evolutionary Algorithms
• Antinuclei from Primordial Black Holes
• Astrophysical or Terrestrial: Machine learning classification of gravitational-wave candidates using multiple-search information
• A two-step strategy to identify episodic sources of gravitational waves and high energy neutrinos in starburst galaxies
• Effectiveness of Stacks in the Stacked Hilbert-Huang Transform
• A Robust and Efficient F-statistic-based Framework for Consistent Bayesian Inference of Compact Binary Coalescences
• Impact of Detector Calibration Accuracy on Black Hole Spectroscopy
• Search for planetary-mass ultra-compact binaries using data from the first part of the LIGO--Virgo--KAGRA fourth observing run
• Apparent horizon as a membrane
• Auto-encoder model for faster generation of effective one-body gravitational waveform approximations
• Measuring spin precession from massive black hole binaries with gravitational waves: insights from time-domain signal morphology
• Physics beyond the Standard Model with the DSA-2000
• Evaluating statistical significance for massive black hole binary mergers with space-based gravitational wave detectors
• Prospects for Neutrino Observation and Mass Measurement from Binary Neutron Star Mergers
• Similar Fermi-GBM sGRBs to GW/sGRB 170817A in MeV-GeV energies
• Shaken, not stirred: Test particles in binary black hole mergers
• The Missing Multipole Problem: Investigating biases from model starting frequency in gravitational-wave analyses
• Enhancing the significance of astrophysical events with multimessenger coincidences
• Probing higher curvature gravity via ringdown with overtones
• Distinguishing between Black Holes and Neutron Stars within a Population of Weak Tidal Measurements
• Global time-frequency search for stellar-mass binary black holes in LISA
• Spin and flavor oscillations of neutrinos in gravitational fields
• Trends in gravitational wave emission in axisymmetric simulations of rotating core-collapse supernovae
• Precision Joint Constraints on Cosmology and Gravity Using Strongly Lensed Gravitational Wave Populations
• Gravitational waves from a binary source in higher dimensional spacetime with compactified extra dimensions
• Black-hole ringdown with templates capturing spin precession: A reanalysis of GW190521
• Identification of time-correlated neutrino clusters in populations of astrophysical transient sources
• Examining the Gap in the Chirp Mass Distribution of Binary Black Holes
• There and back again: Outspiraling motion in non-Kerr compact objects
• Across the Universe: GW231123 as a magnified and diffracted black hole merger
• Gravitational lensing of gravitational waves: universal characteristics of strongly lensed memory waveforms
• Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing?
• Predictions on observing hot holographic quark star with gravitational waves
• Rapid sinking and efficient mergers of supermassive black holes in compact high-redshift galaxies
• A simple example of "non-minimal" Pre-Big Bang scenario
• Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition
• Reducing suspension control noise with interferometric sensors -- an experimental concept
• MaxWave: Rapid maximum likelihood wavelet reconstruction of non-Gaussian features in gravitational wave data
• Beyond general relativity: gravitational waves in non-minimally coupled theories
• Constraining Lorentz and parity violations in gravity with multiband gravitational wave observations
• A Study of Systematics on the Cosmological Inference of the Hubble Constant from Gravitational Wave Standard Sirens
• Detecting White Dwarf Binary Mergers with Gravitational Waves
• Where are Gaia's small black holes?
• Dynamical system approach to the spectral (in)stability of black holes under localised potential perturbations
• Formation of massive multiple-star systems: early migration and mergers
• Robust Bilinear-Noise-Optimal Control for Gravitational-Wave Detectors: A Mixed LQG/$H_{\infty }$ Approach
• Searches for Compact Binary Coalescence Events Using Neural Networks in LIGO/Virgo Third Observation Period
• Constraining gravitational wave velocities using gravitational and electromagnetic wave observations of white dwarf binaries
• Assessment of normalizing flows for parameter estimation on time-frequency representations of gravitational-wave data
• Effects of local cosmic inhomogeneities on the gravitational wave event rate
• Single-rotating Five-dimensional Near-horizon Extremal Geometry in General Relativity
• Impact of facility timing and coordination for next-generation gravitational-wave detectors
• Population Properties of Binary Black Holes with Eccentricity
• Shadows of Giants: Constraints on Stupendously Large Black Holes from Negative Sources against the Cosmic Microwave Background
• Modern tidal interaction models for rapid binary population synthesis: I. Methods
• Uncovering subdominant multipole asymmetries in binary black-hole mergers
• Gravitational-wave constraints on noncommutative spacetime from GW190814
• Circularly polarized gravitational waves from parity-violating scalar-tensor theory
• Lightweight posterior construction for gravitational-wave catalogs with the Kolmogorov-Arnold network
• Quasinormal spectra of a wormhole family: overtone features and a parameter-controlled redshift
• 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
• Comparing a Compact-Binary Mass-Shell Model with Select Observed Gravitational Waves
• High Sensitivity Methodologies to Detect Radio Band Gravitational Waves
• Scattering from compact objects: Debye series and Regge-Debye poles
• Multi-detector characterization of gravitational-wave burst tensor polarizations with the BayesWave algorithm
• Constraining Scalar Charge in Neutron Stars through Gravitational Wave Signals from NSBH Mergers
• Testing classical-quantum gravity with geodesic deviation
• Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge
• Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz
• Uncertainty in predicting the stochastic gravitational wave background from compact binary coalescences
• Las Cumbres Observatory Gravitational-Wave Follow-up in the Third and Fourth Observing Runs: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy
• Smoluchowski Coagulation Equation and the Evolution of Primordial Black Hole Clusters
• Joint Detection and Characterization of the Standing Accretion Shock Instability for Core-Collapse Supernovae with cWB XP
• Improved Constraints on Non-Kerr Deviations from Binary Black Hole Inspirals Using GWTC-4 Data
• Linear perturbations of dyonic black holes in the lowest-order $U(1)$ gauge-invariant scalar-vector-tensor theories
• Enhancing gravitational-wave detection: a machine learning pipeline combination approach with robust uncertainty quantification
• Could the high-mass black holes from gravitational-wave observations be explained by lensing?
• Gravitational-wave astronomy requires population-informed parameter estimation
• Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves
• Multimessenger Signatures of Tilted, Self-Gravitating, Black Hole Disks
• The Role of High-mass Stellar Binaries in the Formation of High-mass Black Holes in Dense Star Clusters
• The maximum mass and rotational kinetic energy of rapidly rotating neutron stars
• Search for gravitational-wave bursts in LIGO data at the Schenberg antenna sensitivity range
• Inferring host environment properties and gravitational-wave decay time from the eccentricity measurement of dynamically captured binaries
• Primordial black holes from D-parity breaking in SO(10) grand unified theory
• Gravitational wave astronomy: astrophysical and cosmological inferences
• 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
• Model-agnostic search of gravitational wave echoes in LVK data
• Full analytic expressions of overlap reduction functions for anisotropies of the stochastic gravitational-wave background with pulsar timing arrays
• Massive black holes and their galaxies
• Unveiling gravitational waves from core-collapse supernovae with MUSE
• Gravitational-Wave Signatures of Massive Black Hole Formation
• Extract non-Gaussian Features in Gravitational Wave Observation Data Using Self-Supervised Learning